{"meta":{"query_hash":"9245c631f799","filters":{"venue":"The Astrophysical Journal"},"cohort_total":6334,"direct_labels_cover":0,"predictions_cover":6334,"exported":6334,"export_cap":100000,"truncated":false,"label_status":"direct model label, unvalidated","prediction_status":"machine_predicted_unvalidated (Codex and Gemma teacher distillation)","score_status":"score_only:v0-immature-baseline","snapshot":{"source":"OpenAlex, pinned release, all 482 partitions","release":"2026-06-24","frame_built":"2026-07-12"},"permalink":"https://metacan.xera.ac/q/9245c631f799","api":"https://metacan.xera.ac/api/v1/cohort?venue=The+Astrophysical+Journal"},"results":[{"id":"W136006321","doi":"10.1086/340491","title":"Galactic Starburst NGC 3603 from X‐Rays to Radio","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; ROSAT; Astronomy; Galaxy; Stars; H II region; Star formation; Point source; Galaxy cluster; Cluster (spacecraft)","score_opus":0.01832948398641456,"score_gpt":0.22028398994755424,"score_spread":0.20195450596113967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W136006321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9654049,0.001478592,0.0011782378,0.00025438107,0.000074805306,0.000044720076,0.0044348305,0.0009250644,0.026204415],"genre_scores_gemma":[0.98942953,0.0007252816,0.0012271848,0.00016367364,0.00002030265,0.000010356653,0.004622513,0.000051060335,0.0037501983],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999355,0.000003473087,0.000005453147,0.000019719246,0.000019099904,0.000016788132],"domain_scores_gemma":[0.9998739,0.0000049571668,0.0000444747,0.000017377586,0.00001546404,0.000043762513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000057522106,0.0002591785,0.00013111203,0.00032066493,0.0004882905,0.0005884607,0.00018206309,0.00014128735,0.0045150747],"category_scores_gemma":[0.00013761014,0.00009263872,0.00017409904,0.0005603173,0.00018197233,0.00017992212,0.00045953537,0.00029253325,0.0012997412],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006421373,0.00013332417,0.7249762,0.00032620996,0.00009307154,0.0020481453,0.0018625364,0.00075346656,0.15640001,0.002239335,0.015858267,0.09466731],"study_design_scores_gemma":[0.000014980402,0.00009983863,0.9503477,0.00003521558,0.000024453004,0.0025399267,0.00036018927,0.00014148229,0.0023445934,0.0004962226,0.043585483,0.000009924659],"about_ca_topic_score_codex":0.010238338,"about_ca_topic_score_gemma":0.016671684,"teacher_disagreement_score":0.010238338,"about_ca_system_score_codex":0.0003131635,"about_ca_system_score_gemma":0.00020879229,"threshold_uncertainty_score":0.02035749},"labels":[],"label_agreement":null},{"id":"W1479809817","doi":"10.1088/0004-637x/807/1/88","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. IX. ESTIMATING THE EFFICIENCY OF GALAXY FORMATION ON THE LOWEST-MASS SCALES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Herzberg Institute of Astrophysics; University of Waterloo","funders":"","keywords":"Physics; Virgo Cluster; Astrophysics; Stellar mass; Astronomy; Luminosity function; Galaxy; Initial mass function; Star formation; Surface brightness; Galaxy cluster; Dwarf galaxy; Cluster (spacecraft); Luminosity","score_opus":0.03406273716963245,"score_gpt":0.24386604193056102,"score_spread":0.20980330476092857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1479809817","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07286861,0.0026724986,0.0014575887,0.0022354831,0.00036589286,0.00038507878,0.897335,0.0011670712,0.021512762],"genre_scores_gemma":[0.15907148,0.0012638428,0.007940407,0.00092793244,0.00015266729,0.00079741655,0.8100518,0.00023620666,0.019558305],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996159,0.000067720706,0.000030547617,0.00006581636,0.0001304293,0.00008954671],"domain_scores_gemma":[0.99852836,0.00008283523,0.00022964034,0.00021678492,0.0004792222,0.000463118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012386993,0.00057992974,0.0004237203,0.005213009,0.00074485154,0.0009948555,0.001419366,0.0006071381,0.0067749084],"category_scores_gemma":[0.002431063,0.00031522076,0.00058847584,0.00447875,0.0001970373,0.0006114382,0.0018874741,0.0007189117,0.0042110607],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003487089,0.00012697907,0.31298882,0.00041434445,0.0003003249,0.000113274175,0.00028950893,0.001018894,0.0010560484,0.0027618299,0.6263439,0.054237396],"study_design_scores_gemma":[0.000074132295,0.00002807355,0.89674795,0.000103897655,0.000077481476,0.00006612146,0.000262684,0.0005098725,0.00038530206,0.0007855852,0.10093644,0.00002238304],"about_ca_topic_score_codex":0.2625117,"about_ca_topic_score_gemma":0.28577358,"teacher_disagreement_score":0.2625117,"about_ca_system_score_codex":0.0019618222,"about_ca_system_score_gemma":0.0018181631,"threshold_uncertainty_score":0.5219674},"labels":[],"label_agreement":null},{"id":"W1481951957","doi":"10.1088/0004-637x/812/2/154","title":"DECONSTRUCTING THERMAL SUNYAEV–ZEL’DOVICH—GRAVITATIONAL LENSING CROSS-CORRELATIONS: IMPLICATIONS FOR THE INTRACLUSTER MEDIUM","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Intracluster medium; Cosmic microwave background; Planck; Weak gravitational lensing; Galaxy; Baryon; Galaxy cluster; Halo; Gravitational lens; Dark matter","score_opus":0.023784451901385072,"score_gpt":0.3104959960759709,"score_spread":0.28671154417458583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1481951957","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98190695,0.0006776656,0.014680984,0.00025681403,0.000017173435,0.000010876104,0.00019875886,0.00010533015,0.002145508],"genre_scores_gemma":[0.99847656,0.00012539068,0.0010683644,0.00003174681,0.000021897333,0.0000042355855,0.0001343042,0.000016854045,0.00012075011],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999634,0.000100312434,0.000016296271,0.00008600076,0.00007766683,0.00008564636],"domain_scores_gemma":[0.99525094,0.0020877952,0.0013570947,0.0005430836,0.00024720118,0.00051388924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002149032,0.0006946023,0.0005035594,0.0015061564,0.0003859749,0.0016183957,0.0006415567,0.00034561957,0.00062723854],"category_scores_gemma":[0.006090769,0.00036076937,0.00055426673,0.001012413,0.0008997117,0.001166623,0.0011553003,0.00064270786,0.00008117839],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028882528,0.000051128896,0.8764632,0.000106133775,0.0010502856,0.00047058845,0.0005694243,0.03707622,0.018075386,0.033618376,0.0010810505,0.03114934],"study_design_scores_gemma":[0.00002735752,0.0000670096,0.7739174,0.000030384941,0.00010785657,0.00020486035,0.00024254175,0.19700037,0.005065261,0.021864885,0.0014001561,0.0000718906],"about_ca_topic_score_codex":0.008336185,"about_ca_topic_score_gemma":0.008068572,"teacher_disagreement_score":0.008336185,"about_ca_system_score_codex":0.00076758093,"about_ca_system_score_gemma":0.00042304146,"threshold_uncertainty_score":0.016575336},"labels":[],"label_agreement":null},{"id":"W1482619730","doi":"10.1086/505907","title":"Detection of Diffuse Interstellar Bands in the <i>z</i>  = 0.5 Damped Lyα System toward AO 0235+164","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Redshift; Measure (data warehouse); Galaxy; Extinction (optical mineralogy); Equivalent width; Spectral line","score_opus":0.007721675245412277,"score_gpt":0.20840776836020705,"score_spread":0.20068609311479477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1482619730","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987061,0.00012798567,0.00016047091,0.0000127494895,0.0000031610273,0.000003002366,0.000045264063,0.000018440089,0.000922779],"genre_scores_gemma":[0.99947757,0.000029655263,0.00021846546,0.000021147425,0.000003827608,0.0000017285089,0.00008743474,0.000001996273,0.00015825668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990225,0.0000053892973,0.000004523401,0.000028871726,0.000032924625,0.000026022184],"domain_scores_gemma":[0.9997111,0.000017107572,0.0001153837,0.0000209185,0.0000360593,0.000099334065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012821953,0.0002098671,0.00013766644,0.000633477,0.00032061845,0.00045593153,0.00032604823,0.00027982038,0.0008974556],"category_scores_gemma":[0.00026019462,0.00017394638,0.00010032541,0.00038387722,0.0003398089,0.00017217119,0.0005172752,0.0002751807,0.00021448858],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022041643,0.00006780375,0.6471188,0.00006560023,0.000081808925,0.0006512824,0.0007394652,0.00017656933,0.33442828,0.00060317374,0.0003684062,0.015478269],"study_design_scores_gemma":[0.00001062391,0.00012507281,0.9932828,0.000005481518,0.000026037062,0.00045078155,0.00012473867,0.00017440518,0.004677366,0.00009565414,0.0010216185,0.0000053608082],"about_ca_topic_score_codex":0.0026808146,"about_ca_topic_score_gemma":0.0056283753,"teacher_disagreement_score":0.0026808146,"about_ca_system_score_codex":0.00026911558,"about_ca_system_score_gemma":0.000116539886,"threshold_uncertainty_score":0.0053304434},"labels":[],"label_agreement":null},{"id":"W1482987092","doi":"10.1088/0004-637x/806/2/189","title":"LINKING GALAXIES TO DARK MATTER HALOS AT<i>z</i>∼ 1: DEPENDENCE OF GALAXY CLUSTERING ON STELLAR MASS AND SPECIFIC STAR FORMATION RATE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council; National Research Foundation of Korea; Centre National de la Recherche Scientifique; Ministry of Science, ICT and Future Planning; National Research Foundation","keywords":"Galaxy; Stellar mass; Luminous infrared galaxy; Halo; Satellite galaxy; Galaxy formation and evolution; Star formation; Galaxy group; Dark matter","score_opus":0.015520279431271336,"score_gpt":0.21455406834680138,"score_spread":0.19903378891553003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1482987092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992944,0.000052422598,0.00019016316,0.000018935703,6.2726195e-7,0.0000018691095,0.00014040284,0.000021614778,0.00027954654],"genre_scores_gemma":[0.99956006,0.000019614481,0.000090899404,0.0000051509614,0.0000026740222,0.0000010125553,0.00025024783,0.0000052814216,0.00006508455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998159,0.000030135852,0.0000075364637,0.000055980374,0.000022408993,0.00006805898],"domain_scores_gemma":[0.99616843,0.0012027181,0.0013305545,0.00031213925,0.00030045293,0.00068569503],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004959804,0.0002921311,0.0002657373,0.0016327796,0.0002204436,0.00080525223,0.00033675772,0.00045844246,0.0011837025],"category_scores_gemma":[0.002553607,0.0002902206,0.00037596852,0.0009888451,0.00038929738,0.00040429723,0.0005796139,0.00033379137,0.00033731165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006830507,0.000019922694,0.9928289,0.0000074376558,0.000055154676,0.00006076743,0.00013340196,0.002231995,0.0023666269,0.00020815237,0.000110006535,0.0019094561],"study_design_scores_gemma":[0.0000021810508,0.000011299361,0.9944593,0.0000026661037,0.000011533896,0.00003266135,0.000050638195,0.005052296,0.00020812864,0.000104123246,0.00006005491,0.000005133407],"about_ca_topic_score_codex":0.012058448,"about_ca_topic_score_gemma":0.009390354,"teacher_disagreement_score":0.012058448,"about_ca_system_score_codex":0.0003429547,"about_ca_system_score_gemma":0.00014507968,"threshold_uncertainty_score":0.023976505},"labels":[],"label_agreement":null},{"id":"W1484263073","doi":"10.1088/0004-637x/716/1/348","title":"THE<i>XMM-NEWTON</i>WIDE-FIELD SURVEY IN THE COSMOS FIELD (XMM-COSMOS): DEMOGRAPHY AND MULTIWAVELENGTH PROPERTIES OF OBSCURED AND UNOBSCURED LUMINOUS ACTIVE GALACTIC NUCLEI","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":281,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Redshift; Active galactic nucleus; Cosmos (plant); Population; Flux (metallurgy); Hubble Deep Field; Infrared; Quasar","score_opus":0.015138267695845593,"score_gpt":0.2233685989097054,"score_spread":0.2082303312138598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1484263073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6768146,0.017225657,0.0146491295,0.0014709345,0.00031495697,0.00037752054,0.25589973,0.0027613686,0.03048607],"genre_scores_gemma":[0.5178402,0.009948595,0.061494455,0.0008213551,0.0006514553,0.00040195519,0.39917392,0.0005819793,0.009086107],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978787,0.000023034205,0.00001592939,0.00007349495,0.000060147628,0.000039401635],"domain_scores_gemma":[0.99890447,0.00006201965,0.00041675585,0.00023001357,0.00015057996,0.00023607483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006618595,0.0006727047,0.00025349742,0.0048740413,0.00035336736,0.00086441997,0.00036130735,0.00022360263,0.00225648],"category_scores_gemma":[0.0006820539,0.00023229225,0.0002905049,0.0035048253,0.00026316353,0.0007031297,0.0012509074,0.00037379473,0.0018055066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019260886,0.00014329933,0.70588756,0.0004985908,0.00020536942,0.00031951847,0.00035589104,0.0008466688,0.023059834,0.003045677,0.05245965,0.21298541],"study_design_scores_gemma":[0.000009327016,0.00004489457,0.90532875,0.000051150284,0.000031080806,0.00027051326,0.000054308293,0.00025719305,0.003687233,0.00047791706,0.08977089,0.000016776467],"about_ca_topic_score_codex":0.006808841,"about_ca_topic_score_gemma":0.012264896,"teacher_disagreement_score":0.006808841,"about_ca_system_score_codex":0.00040290807,"about_ca_system_score_gemma":0.00060425827,"threshold_uncertainty_score":0.01353842},"labels":[],"label_agreement":null},{"id":"W1484483366","doi":"10.3847/1538-4357/aa6c68","title":"The Mass–Concentration Relation and the Stellar-to-halo Mass Ratio in the CFHT Stripe 82 Survey","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Waterloo; University of British Columbia","funders":"","keywords":"Galaxy; Weak gravitational lensing; Sky; Dark matter; Baryon; Galaxy cluster; Telescope; South Pole Telescope; Cluster (spacecraft)","score_opus":0.011404840140413892,"score_gpt":0.22790195702211688,"score_spread":0.21649711688170298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1484483366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982167,0.000022336206,0.00011517486,0.000020538904,7.558453e-7,0.0000023066812,0.00066790235,0.000011438263,0.0009427694],"genre_scores_gemma":[0.9989454,0.000010818095,0.00009610125,0.000009179289,0.0000033478714,0.0000024059784,0.0007908799,0.0000028528682,0.00013907457],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972445,0.00004205487,0.000014875114,0.00007320999,0.000074386,0.00007098916],"domain_scores_gemma":[0.9983228,0.0002325672,0.0005640087,0.0002449008,0.00038462033,0.00025114013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005301274,0.00016073958,0.00015725833,0.0016187078,0.00027534002,0.00041983556,0.00022653845,0.00022093873,0.0013528656],"category_scores_gemma":[0.0018060395,0.00010176443,0.00012619617,0.0010895468,0.00043196493,0.00034637444,0.00048339315,0.00013225658,0.00031478767],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003701923,0.000009643946,0.993284,0.0000049771156,0.000019888346,0.000029230938,0.000118828364,0.0003322938,0.0035472028,0.00014681659,0.0004061028,0.00206388],"study_design_scores_gemma":[0.0000018631177,0.0000053156637,0.99907255,0.000001046861,0.0000021882493,0.000013235854,0.000029542833,0.00045060867,0.00028490307,0.000019595345,0.00011725562,0.000001884021],"about_ca_topic_score_codex":0.04498634,"about_ca_topic_score_gemma":0.055604376,"teacher_disagreement_score":0.04498634,"about_ca_system_score_codex":0.0006369043,"about_ca_system_score_gemma":0.00022679433,"threshold_uncertainty_score":0.08944899},"labels":[],"label_agreement":null},{"id":"W1487858455","doi":"10.1088/0004-637x/703/2/l104","title":"SIGNATURES OF RELATIVISTIC HELICAL MOTION IN THE ROTATION MEASURES OF ACTIVE GALACTIC NUCLEUS JETS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Transverse plane; Polarization (electrochemistry); Bent molecular geometry; Toroid; Magnetic field; Active galactic nucleus; Jet (fluid); Astrophysical jet","score_opus":0.014122332103775644,"score_gpt":0.24046120171743557,"score_spread":0.22633886961365993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1487858455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99288625,0.00023757844,0.005311365,0.000030643172,0.000008387416,0.0000044259323,0.00016907127,0.00013078714,0.0012213825],"genre_scores_gemma":[0.99906343,0.00004249693,0.0007230599,0.0000034319537,0.0000056329063,0.0000020027076,0.00007528534,0.000012662827,0.00007209212],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999548,0.000009337876,0.000003532508,0.000012920341,0.000009178405,0.000010130118],"domain_scores_gemma":[0.99955314,0.000093113595,0.00022450705,0.00007151963,0.000027205344,0.000030569652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001966034,0.0001789121,0.00011544864,0.00080583326,0.00013711308,0.000462968,0.00016445229,0.00018114345,0.00052491395],"category_scores_gemma":[0.0008400741,0.0001745991,0.00013797816,0.00043740548,0.00024042754,0.00017462706,0.00017177583,0.00014881081,0.00012524193],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008756967,0.00008617882,0.37243086,0.0001162166,0.000102138634,0.000780873,0.0006223499,0.021464325,0.5381046,0.006461591,0.0007247344,0.058230463],"study_design_scores_gemma":[0.000031886462,0.00009881164,0.92536646,0.000014718249,0.000042315074,0.00066955166,0.000083964864,0.043791257,0.026080988,0.0026748592,0.0011071367,0.000038092592],"about_ca_topic_score_codex":0.00070855743,"about_ca_topic_score_gemma":0.00071963866,"teacher_disagreement_score":0.00080583326,"about_ca_system_score_codex":0.0001938877,"about_ca_system_score_gemma":0.000056971334,"threshold_uncertainty_score":0.0017560124},"labels":[],"label_agreement":null},{"id":"W1492354913","doi":"10.1088/0004-637x/744/2/89","title":"SEARCH FOR<i>z</i>∼ 7 Lyα EMITTERS WITH THE SUPRIME-CAM AT THE SUBARU TELESCOPE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Subaru Telescope; Luminosity; Luminosity function; Telescope; Measure (data warehouse); William Herschel Telescope; Quasar; Range (aeronautics)","score_opus":0.013387314470051684,"score_gpt":0.21117390361710583,"score_spread":0.19778658914705416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1492354913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99630547,0.00017898383,0.0020414472,0.000031745647,0.000004211537,0.000014544267,0.00020264665,0.00007297833,0.0011480573],"genre_scores_gemma":[0.9888204,0.00012317268,0.00931529,0.0000655214,0.00003623059,0.000024361654,0.001067037,0.000027805516,0.0005203111],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997476,0.00002813843,0.000011980201,0.00007482522,0.000072489616,0.000064936474],"domain_scores_gemma":[0.9988952,0.0002149349,0.000341082,0.00017080778,0.00014286558,0.00023515767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009968341,0.00035248432,0.00048854796,0.0014157871,0.000504161,0.00052233634,0.000724388,0.00035830378,0.0009755373],"category_scores_gemma":[0.00056211057,0.00037040125,0.000517285,0.00078569737,0.00020377834,0.000329499,0.00043018232,0.0003656871,0.00055995985],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006678944,0.00021636403,0.78534997,0.000063280604,0.00016582926,0.0004591772,0.00037828798,0.0004287114,0.18172272,0.00050492253,0.0007253317,0.029317519],"study_design_scores_gemma":[0.00004061171,0.0005778504,0.9703939,0.000010065484,0.00014037045,0.00084073126,0.00009634574,0.0022250665,0.022994045,0.00023229966,0.0024346435,0.000014127907],"about_ca_topic_score_codex":0.00053126505,"about_ca_topic_score_gemma":0.0014155937,"teacher_disagreement_score":0.0014157871,"about_ca_system_score_codex":0.00017118573,"about_ca_system_score_gemma":0.00015200475,"threshold_uncertainty_score":0.0052717924},"labels":[],"label_agreement":null},{"id":"W1495799903","doi":"10.1088/0004-637x/693/1/56","title":"SMA<sup>12</sup>CO(<i>J</i>= 6 – 5) AND 435 μm INTERFEROMETRIC IMAGING OF THE NUCLEAR REGION OF Arp 220","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Toronto","funders":"","keywords":"Physics; Interferometry; Wavelength; Nucleus; Emissivity; Astrophysics; Submillimeter Array; Excitation; Emission spectrum; Line (geometry); Spectral line; Atomic physics; Astronomy; Optics; Star formation; Galaxy","score_opus":0.009245722522376666,"score_gpt":0.22166157755933782,"score_spread":0.21241585503696117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1495799903","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99029934,0.00017654664,0.002866709,0.0000573954,0.000014609337,0.000010514746,0.0012001193,0.00020462199,0.0051700887],"genre_scores_gemma":[0.9825682,0.000084997686,0.013914497,0.000053929904,0.000029970488,0.00001313184,0.002343023,0.00004760228,0.00094463857],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999039,0.0000074247914,0.000003034554,0.000024863712,0.000036052705,0.000024828334],"domain_scores_gemma":[0.9997725,0.000017188644,0.0000772654,0.00003701695,0.000041517946,0.000054607997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021180457,0.00014404625,0.00010120074,0.00045846976,0.00021716126,0.00030986426,0.0002680207,0.00014920167,0.001225306],"category_scores_gemma":[0.0002096375,0.00017889128,0.00015846673,0.00033486454,0.0001029794,0.00019407469,0.00022624919,0.00020758143,0.00048033157],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039475094,0.00015649006,0.1810866,0.00009603048,0.00010707397,0.0005567828,0.00026273646,0.0026820186,0.75984484,0.000744684,0.0021460466,0.051921923],"study_design_scores_gemma":[0.00001346948,0.00012763981,0.93705267,0.00000960022,0.00005547565,0.00056384446,0.000110416615,0.0046182033,0.05107469,0.00017297869,0.006186222,0.000014770521],"about_ca_topic_score_codex":0.0026102406,"about_ca_topic_score_gemma":0.008702359,"teacher_disagreement_score":0.0026102406,"about_ca_system_score_codex":0.00018102342,"about_ca_system_score_gemma":0.0001545793,"threshold_uncertainty_score":0.005190134},"labels":[],"label_agreement":null},{"id":"W1496380348","doi":"10.3847/0004-637x/820/1/11","title":"CONFIRMING THE EXISTENCE OF A QUIESCENT GALAXY POPULATION OUT TO z = 3: A STACKING ANALYSIS OF MID-, FAR-INFRARED, AND RADIO DATA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mount Allison University","funders":"","keywords":"Stacking; Galaxy; Redshift; Population; Star formation; Radio galaxy; Milky Way","score_opus":0.025085542639764532,"score_gpt":0.26245073157432564,"score_spread":0.2373651889345611,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1496380348","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988673,0.000060379818,0.00044173258,0.0000050936746,8.7368926e-7,0.0000047123126,0.00033551926,0.000021910768,0.00026272383],"genre_scores_gemma":[0.99848807,0.000017038963,0.0004928355,0.000007944785,0.0000033608394,0.0000031121242,0.00091885024,0.00000465457,0.000064156266],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968934,0.00003339711,0.000024830844,0.00008024168,0.000064174055,0.000108137116],"domain_scores_gemma":[0.9987379,0.00017337865,0.00033334718,0.00017451831,0.00019832439,0.00038255908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005844547,0.0002717206,0.00038621947,0.0020916974,0.00054150424,0.00063238456,0.00026656632,0.00015055276,0.0012740605],"category_scores_gemma":[0.00087258493,0.00012328473,0.0004298997,0.00122151,0.00028901617,0.0002931637,0.00077418715,0.00019009224,0.0003528185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008852888,0.000023072016,0.9699715,0.000014992443,0.0000656728,0.00012148913,0.0002432965,0.00035500756,0.020485755,0.00010296577,0.0001534831,0.008374277],"study_design_scores_gemma":[0.0000012896522,0.000029197097,0.99806434,0.0000014542354,0.000022933025,0.000054216835,0.000074283234,0.00052739365,0.001013071,0.00003070022,0.00017847258,0.0000027221577],"about_ca_topic_score_codex":0.0056206817,"about_ca_topic_score_gemma":0.00712387,"teacher_disagreement_score":0.0056206817,"about_ca_system_score_codex":0.0002044139,"about_ca_system_score_gemma":0.00019710777,"threshold_uncertainty_score":0.0111759305},"labels":[],"label_agreement":null},{"id":"W1496472807","doi":"10.1088/0004-637x/714/1/825","title":"GALAXY COUNTS ON THE COSMIC MICROWAVE BACKGROUND COLD SPOT","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Cosmic microwave background; Astrophysics; Physics; Redshift; Galaxy; Sky; RADIUS; Astronomy; COSMIC cancer database; Cold dark matter; Cosmic variance; Universe; Optics","score_opus":0.010390666329569745,"score_gpt":0.21545650882141865,"score_spread":0.2050658424918489,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1496472807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.991888,0.00013872006,0.00049361156,0.000039128197,0.000006233815,0.0000054802194,0.0010131989,0.000099973775,0.006315616],"genre_scores_gemma":[0.99790025,0.000042451862,0.00034473927,0.000023596987,0.000013684503,0.0000046663595,0.0010609733,0.00001199705,0.0005976074],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973625,0.0000458373,0.000013728298,0.000061012473,0.000078781435,0.00006444921],"domain_scores_gemma":[0.9987685,0.0002502288,0.00025131335,0.00018838106,0.00023411424,0.00030744253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028482926,0.0001562947,0.00024092663,0.0015290756,0.00017605268,0.00037529098,0.00021670453,0.00017847642,0.0028979366],"category_scores_gemma":[0.0015101129,0.00010750477,0.00012262675,0.00094438414,0.00028240914,0.00024823457,0.00042979437,0.00022357874,0.00050626736],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032365497,0.00003462531,0.94358814,0.000056022138,0.0000976572,0.00020040135,0.00037739362,0.0006086025,0.027466748,0.0017246203,0.002221906,0.023300223],"study_design_scores_gemma":[0.000002799672,0.000019715359,0.99737763,0.000002962841,0.00000975752,0.00013547408,0.000026747784,0.00031229324,0.001316082,0.000108774824,0.00068489154,0.0000029249625],"about_ca_topic_score_codex":0.0021923939,"about_ca_topic_score_gemma":0.0031835274,"teacher_disagreement_score":0.0028979366,"about_ca_system_score_codex":0.00024380935,"about_ca_system_score_gemma":0.00006230635,"threshold_uncertainty_score":0.009694576},"labels":[],"label_agreement":null},{"id":"W1497063077","doi":"10.1088/0004-637x/811/1/30","title":"THE SYNTHETIC-OVERSAMPLING METHOD: USING PHOTOMETRIC COLORS TO DISCOVER EXTREMELY METAL-POOR STARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Stars; Sky; Broadband; False positive paradox; Apparent magnitude; Stellar evolution; Photometry (optics); Cosmology","score_opus":0.05038566446886786,"score_gpt":0.3000201767849847,"score_spread":0.24963451231611686,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1497063077","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34853247,0.00053451076,0.64258647,0.00030166644,0.000118457494,0.00009505129,0.00082580687,0.0045191315,0.002486497],"genre_scores_gemma":[0.7520538,0.00013427598,0.24388754,0.00021427387,0.00008868492,0.000057207275,0.0021476906,0.00023940775,0.0011771214],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994943,0.00013241371,0.000022744453,0.00018103282,0.00012193767,0.000047576425],"domain_scores_gemma":[0.9981194,0.00048812808,0.00028393287,0.0006921426,0.0003097095,0.000106617794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015024014,0.00066779135,0.00045910894,0.0011742578,0.00045397785,0.0007124878,0.0011758473,0.0006014036,0.00075022824],"category_scores_gemma":[0.0054849526,0.00029665206,0.00068385294,0.00065455283,0.0005326873,0.00055621134,0.001005811,0.00058557926,0.00047653203],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008966865,0.0003465718,0.1541338,0.00017493087,0.0005858043,0.00027327932,0.00032981526,0.23144186,0.06734209,0.008845785,0.008622429,0.527007],"study_design_scores_gemma":[0.000045956465,0.00008072283,0.020276431,0.000014578765,0.00006883596,0.0003338292,0.00005688933,0.9457251,0.022545163,0.006820135,0.003982904,0.0000494051],"about_ca_topic_score_codex":0.004117476,"about_ca_topic_score_gemma":0.0051182117,"teacher_disagreement_score":0.004117476,"about_ca_system_score_codex":0.00045750584,"about_ca_system_score_gemma":0.0007296264,"threshold_uncertainty_score":0.008187056},"labels":[],"label_agreement":null},{"id":"W1498296330","doi":"10.1088/0004-637x/712/2/1057","title":"SUPERNOVA 1986J VERY LONG BASELINE INTERFEROMETRY. II. THE EVOLUTION OF THE SHELL AND THE CENTRAL SOURCE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Very-long-baseline interferometry; Supernova; Opacity; Proper motion; Shock (circulatory); Center (category theory)","score_opus":0.004548880991377774,"score_gpt":0.19638455301268404,"score_spread":0.19183567202130627,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1498296330","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98932636,0.0004245726,0.0028420188,0.000051401978,0.000016309761,0.000022495173,0.0035495858,0.0001590123,0.0036083146],"genre_scores_gemma":[0.9853172,0.00020412562,0.005178681,0.000039329712,0.000018646218,0.000018487975,0.007807473,0.000022823373,0.001393245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992263,0.000006008885,0.0000035731534,0.000019639607,0.000022249007,0.000025897072],"domain_scores_gemma":[0.9998511,0.000009408593,0.000059072554,0.00002086293,0.000023632638,0.000035860354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019438971,0.00024406545,0.00016051061,0.0006936864,0.0002337836,0.00037493336,0.0002059481,0.0002141365,0.0011276277],"category_scores_gemma":[0.00021211013,0.00022511845,0.00018809078,0.00048284742,0.00011685804,0.00022940214,0.0002806398,0.00026598544,0.0005083016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005322543,0.00015892649,0.7056466,0.00011813286,0.000136442,0.0005157546,0.00018817095,0.0019673768,0.26084447,0.00089818006,0.002021717,0.02697195],"study_design_scores_gemma":[0.000005780215,0.000019491492,0.9937937,0.0000029382459,0.000011403589,0.00034291483,0.000017178705,0.0010449555,0.003323014,0.00004664951,0.0013874735,0.00000431613],"about_ca_topic_score_codex":0.0049688797,"about_ca_topic_score_gemma":0.011502254,"teacher_disagreement_score":0.0049688797,"about_ca_system_score_codex":0.00033136358,"about_ca_system_score_gemma":0.00014515704,"threshold_uncertainty_score":0.009879947},"labels":[],"label_agreement":null},{"id":"W1501328950","doi":"10.1086/516734","title":"Discovery of a Bipolar Outflow from 2MASSW J1207334-393254, a 24 <i>M</i> <sub>Jup</sub> Brown Dwarf","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Brown dwarf; Physics; Outflow; Bipolar outflow; Circumbinary planet; Astronomy; Radial velocity; Proper motion; Planet; Stars; Star formation","score_opus":0.008885719944077688,"score_gpt":0.21978562217818484,"score_spread":0.21089990223410715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1501328950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99834275,0.000092276394,0.00012246317,0.000052491785,0.000010500839,0.000008333064,0.00025622264,0.000023093577,0.0010919225],"genre_scores_gemma":[0.997703,0.00007555169,0.00047887745,0.00007957112,0.000015247786,0.000006226545,0.0008478529,0.0000071020518,0.00078669516],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993277,0.0000026060716,0.0000036939775,0.000022071687,0.000020998039,0.000017839831],"domain_scores_gemma":[0.9998498,0.000007944216,0.000045021774,0.000008738922,0.000013603692,0.00007484587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000082756225,0.00020743463,0.00022995002,0.00048742298,0.000577254,0.00041121765,0.00027089624,0.0007163867,0.0010446018],"category_scores_gemma":[0.0002352621,0.00014518194,0.0001512528,0.00040205437,0.0002490292,0.00021404016,0.0004822366,0.00025800345,0.00046567273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048456824,0.00016467285,0.5519913,0.00012203311,0.00006487332,0.046026517,0.0012661493,0.00023329075,0.3654122,0.0007142047,0.0021159612,0.031404343],"study_design_scores_gemma":[0.0000227276,0.0003008216,0.9700261,0.000025975422,0.000026201202,0.015071901,0.000511148,0.0005095535,0.007891724,0.00023070113,0.005363645,0.000019522715],"about_ca_topic_score_codex":0.0044861184,"about_ca_topic_score_gemma":0.008488172,"teacher_disagreement_score":0.0044861184,"about_ca_system_score_codex":0.00031047995,"about_ca_system_score_gemma":0.00019417834,"threshold_uncertainty_score":0.008920014},"labels":[],"label_agreement":null},{"id":"W1501391255","doi":"10.1086/318870","title":"The Origin of M[CLC]n[/CLC] [CSC]ii[/CSC] Emission in the Spectra of Chemically Peculiar Stars","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Multiplet; Physics; Astrophysics; Manganese; Stars; Photosphere; Spectral line; Emission spectrum; Radiative transfer; Astronomy; Chemistry; Optics","score_opus":0.01042079892433294,"score_gpt":0.23601171831569956,"score_spread":0.2255909193913666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1501391255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98882467,0.00045313043,0.0017573443,0.00013797403,0.000023489505,0.000010779046,0.00023781144,0.00014074269,0.008414107],"genre_scores_gemma":[0.99866164,0.000057891593,0.00045634253,0.000032420026,0.000007466568,0.000003651795,0.00017392515,0.000018767585,0.0005878352],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99986756,0.000008097478,0.0000052565865,0.000062948,0.000025006459,0.000031066866],"domain_scores_gemma":[0.99976593,0.000017961773,0.00007776907,0.000023703393,0.00003814537,0.00007642024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012169637,0.00022079892,0.00014004156,0.0004593173,0.00032357435,0.00041240125,0.0003379195,0.0003548803,0.0031148558],"category_scores_gemma":[0.00024539616,0.00014927483,0.00013601908,0.00046512616,0.00044637156,0.00021309449,0.00035644407,0.00022404629,0.00032725435],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034655104,0.000077234086,0.18708453,0.00012018714,0.000082072445,0.00046774774,0.0002186675,0.00043310618,0.79063696,0.002795188,0.0009391077,0.016798683],"study_design_scores_gemma":[0.000021355445,0.000076299184,0.92762077,0.000020362046,0.000040991486,0.00069876487,0.00015245327,0.0030813755,0.06123215,0.0011440432,0.005894342,0.000017072321],"about_ca_topic_score_codex":0.00368618,"about_ca_topic_score_gemma":0.006583809,"teacher_disagreement_score":0.00368618,"about_ca_system_score_codex":0.00049195206,"about_ca_system_score_gemma":0.000219603,"threshold_uncertainty_score":0.010420203},"labels":[],"label_agreement":null},{"id":"W1507923592","doi":"10.1086/321340","title":"X‐Ray Observations of the New Pulsar–Supernova Remnant System PSR J1119−6127 and Supernova Remnant G292.2−0.5","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; ROSAT; Supernova remnant; Astrophysics; Millisecond pulsar; Astronomy; Pulsar planet; Supernova; Spectral index; Point source; Near-Earth supernova; Binary pulsar; Spectral line; Galaxy; Optics","score_opus":0.02329116920927905,"score_gpt":0.2876628957572271,"score_spread":0.26437172654794805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1507923592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99828786,0.0000494756,0.000067745576,0.000008509814,0.0000015716041,0.000011240561,0.0008404345,0.000012969321,0.0007201861],"genre_scores_gemma":[0.9875693,0.000157499,0.00080138136,0.000017204984,0.000009412846,0.000024627121,0.010399069,0.000011580825,0.0010098978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998361,0.000013990906,0.000014602701,0.00003641063,0.00006574691,0.00003308473],"domain_scores_gemma":[0.99953735,0.00003553838,0.00017425921,0.00005577435,0.00006326164,0.00013386182],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024515178,0.00022834225,0.00029128202,0.0010981173,0.0004955142,0.0003337185,0.00029284638,0.00022066022,0.0011797666],"category_scores_gemma":[0.00037499148,0.00021938284,0.00016748848,0.0009822147,0.00025253778,0.00019249234,0.00053043873,0.0002567209,0.0005790449],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006571982,0.00047265456,0.8589931,0.00009504848,0.00018079364,0.0018460252,0.00072798994,0.00086693134,0.119452,0.00059241324,0.0020558394,0.014060028],"study_design_scores_gemma":[0.000020015563,0.0000891338,0.99518305,0.0000030156361,0.000019873838,0.00047042026,0.00008259275,0.00029324848,0.001959097,0.00003651787,0.0018374865,0.0000054664633],"about_ca_topic_score_codex":0.005598806,"about_ca_topic_score_gemma":0.017227117,"teacher_disagreement_score":0.005598806,"about_ca_system_score_codex":0.00035343034,"about_ca_system_score_gemma":0.00025285943,"threshold_uncertainty_score":0.011132479},"labels":[],"label_agreement":null},{"id":"W1508701176","doi":"10.1086/312784","title":"[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of Intrinsic Absorption in the Seyfert 1 Galaxy Markarian 509","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Galaxy; Ionization; Emission spectrum; Spectral line; Ultraviolet; Absorption spectroscopy; Absorption (acoustics); Submillimeter Array; Astronomy; Optics; Star formation; Ion","score_opus":0.01896995126857399,"score_gpt":0.23237659026700497,"score_spread":0.213406638998431,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1508701176","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8703226,0.003045168,0.0018308117,0.0013537913,0.0009234961,0.000053418677,0.036729682,0.00155983,0.08418125],"genre_scores_gemma":[0.86246485,0.00314192,0.0062260143,0.0011370028,0.0011761213,0.000052681153,0.086069524,0.0003545597,0.03937741],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9999517,0.000003773198,0.0000031417178,0.000012412778,0.000017222823,0.000011780618],"domain_scores_gemma":[0.9998994,0.000008170435,0.00004265459,0.000011526316,0.000015232856,0.00002300562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009363985,0.00022161113,0.00015451535,0.0011816466,0.00023814198,0.00037038856,0.00025986513,0.00021806816,0.019671375],"category_scores_gemma":[0.00014485657,0.0000687069,0.00017061863,0.00077189464,0.000089761044,0.00025748764,0.00033398555,0.00019093984,0.0057105836],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012933809,0.00029112265,0.2817186,0.00058698293,0.00032079386,0.0036175286,0.00037944922,0.0014397172,0.18822965,0.002468736,0.3224087,0.19724539],"study_design_scores_gemma":[0.00003139625,0.00018778665,0.8564146,0.0000714267,0.000038895065,0.0015214094,0.00009652776,0.0004980796,0.0044564297,0.0003095277,0.13635857,0.000015438272],"about_ca_topic_score_codex":0.0015330345,"about_ca_topic_score_gemma":0.0033143137,"teacher_disagreement_score":0.019671375,"about_ca_system_score_codex":0.00012158037,"about_ca_system_score_gemma":0.000044069046,"threshold_uncertainty_score":0.06580734},"labels":[],"label_agreement":null},{"id":"W1509168094","doi":"10.1086/319636","title":"MACHO Project Limits on Black Hole Dark Matter in the 1–30 [ITAL]M[/ITAL][TINF]⊙[/TINF] Range","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":343,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gravitational microlensing; Physics; Dark matter; Astrophysics; Halo; Dark matter halo; Galactic halo; Large Magellanic Cloud; Baryonic dark matter; Astronomy; Galaxy","score_opus":0.018486454395769954,"score_gpt":0.24702102897448894,"score_spread":0.22853457457871898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1509168094","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2076441,0.014265637,0.028610988,0.020426199,0.0007682978,0.0002801817,0.07076336,0.0021763756,0.6550648],"genre_scores_gemma":[0.87562764,0.0036614912,0.015554941,0.0026906945,0.0010113548,0.0008325083,0.046727777,0.00059826294,0.053295355],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9980811,0.0005386949,0.000050574683,0.00029019132,0.0006918817,0.0003476151],"domain_scores_gemma":[0.9930061,0.0023017451,0.00059583026,0.0010247887,0.0013764078,0.0016952351],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0061325557,0.0006265267,0.000945093,0.0018121558,0.0011649122,0.0032136329,0.0014680456,0.0017527646,0.021591587],"category_scores_gemma":[0.009848409,0.00030970803,0.00056445977,0.0011340836,0.0009796872,0.003416292,0.006290715,0.0011561486,0.005402389],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0042294916,0.00037960982,0.076778516,0.000705958,0.00024994026,0.00063239376,0.0016374834,0.0054523107,0.0028168363,0.44807425,0.27002156,0.18902162],"study_design_scores_gemma":[0.0004037562,0.0006230956,0.2696694,0.0011560308,0.00015566275,0.0010410461,0.0017128726,0.013639119,0.0038604983,0.34543422,0.36215037,0.00015393288],"about_ca_topic_score_codex":0.010574709,"about_ca_topic_score_gemma":0.010163554,"teacher_disagreement_score":0.021591587,"about_ca_system_score_codex":0.00109762,"about_ca_system_score_gemma":0.0012303623,"threshold_uncertainty_score":0.072230995},"labels":[],"label_agreement":null},{"id":"W1509303056","doi":"10.1086/317319","title":"Evidence for a Long-Period Planet Orbiting ε Eridani","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":274,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia","funders":"","keywords":"Physics; Eccentricity (behavior); Planet; Orbital period; Astrophysics; Orbital eccentricity; Orbital motion; Amplitude; Orbit (dynamics); Orbital elements; Rotation period; Radial velocity; Astronomy; Geodesy; Angular momentum; Stars; Classical mechanics; Geology; Optics","score_opus":0.027515230528038302,"score_gpt":0.26180113349368916,"score_spread":0.23428590296565086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1509303056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9853221,0.00071980007,0.0007146748,0.000105087616,0.000034965273,0.000009617385,0.0005558621,0.000056985173,0.012480834],"genre_scores_gemma":[0.99643916,0.00011142699,0.00074723735,0.000058880854,0.000016211332,0.000004828066,0.00072669436,0.000009970221,0.0018856785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998646,0.000005903626,0.000011573211,0.00005547327,0.00002899746,0.000033526412],"domain_scores_gemma":[0.99935967,0.00008192551,0.0002843524,0.0000826932,0.000090512374,0.00010075837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022449341,0.00025249348,0.0002177316,0.00045976453,0.00044021418,0.0006429915,0.00036972124,0.0004544136,0.0014405765],"category_scores_gemma":[0.00056772487,0.0002043913,0.00014054014,0.00050702,0.0002979343,0.00038200978,0.0005013867,0.00036366066,0.0008467327],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062631135,0.00014837986,0.7985227,0.00019062399,0.00012029088,0.0021864937,0.0006722275,0.00061485264,0.1433435,0.001352354,0.002150689,0.050071638],"study_design_scores_gemma":[0.000010430714,0.00015638547,0.9853483,0.000014235793,0.00002342736,0.0012559342,0.00014129853,0.0004540605,0.0039829877,0.00011332907,0.008491336,0.000008149272],"about_ca_topic_score_codex":0.002596248,"about_ca_topic_score_gemma":0.0056587732,"teacher_disagreement_score":0.002596248,"about_ca_system_score_codex":0.00038023782,"about_ca_system_score_gemma":0.0001803823,"threshold_uncertainty_score":0.0051622987},"labels":[],"label_agreement":null},{"id":"W1511001278","doi":"10.1086/308309","title":"The<i>Hubble Space Telescope</i>Key Project on the Extragalactic Distance Scale. XXVI. The Calibration of Population II Secondary Distance Indicators and the Value of the Hubble Constant","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":275,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Cepheid variable; Physics; Astrophysics; Globular cluster; Cosmic distance ladder; Metallicity; Hubble's law; Galaxy; Red-giant branch; Surface brightness fluctuation; Surface brightness; Luminosity; Stellar population; Stars; Astronomy; Star cluster; Population; RR Lyrae variable; Star formation; Redshift; Lenticular galaxy","score_opus":0.005240528733438563,"score_gpt":0.20544617583179417,"score_spread":0.20020564709835562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1511001278","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.031656265,0.034659024,0.03997073,0.013359975,0.007636108,0.0010963393,0.40706727,0.004340701,0.46021357],"genre_scores_gemma":[0.10376559,0.019318044,0.08140777,0.0013739496,0.0017236294,0.0013768628,0.5405545,0.0008904552,0.24958916],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9994362,0.00008743479,0.000026577902,0.00010191344,0.00027846856,0.00006941706],"domain_scores_gemma":[0.99846977,0.00009738065,0.00038910157,0.00024390467,0.0005793965,0.00022043525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014536094,0.0012844948,0.00044290398,0.002911997,0.00047647452,0.0015491917,0.00089308986,0.00069775374,0.020240085],"category_scores_gemma":[0.0016982001,0.00030575445,0.0002558366,0.003911855,0.0003880872,0.0012950229,0.0013385835,0.0014701652,0.018099377],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011685554,0.00006940928,0.013309712,0.0003078531,0.000035720182,0.000059216345,0.000118339936,0.00044807806,0.0018059053,0.037839793,0.69128805,0.25460106],"study_design_scores_gemma":[0.000032393775,0.00004101366,0.09535121,0.00014447882,0.000009214017,0.00007961283,0.00005432267,0.00064151356,0.00073896546,0.007323186,0.89556295,0.000021053997],"about_ca_topic_score_codex":0.025698565,"about_ca_topic_score_gemma":0.014498844,"teacher_disagreement_score":0.025698565,"about_ca_system_score_codex":0.0022728485,"about_ca_system_score_gemma":0.0018114116,"threshold_uncertainty_score":0.06770986},"labels":[],"label_agreement":null},{"id":"W1516723655","doi":"10.1088/0004-637x/814/1/21","title":"A MULTI-WAVELENGTH MASS ANALYSIS OF RCS2 J232727.6-020437, A ∼3 × 10<sup>15</sup><i>M</i><sub>⊙</sub>GALAXY CLUSTER AT<i>z</i>= 0.7","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal","funders":"FP7 People: Marie-Curie Actions; Smithsonian Astrophysical Observatory; University of Chicago; Comisión Nacional de Investigación Científica y Tecnológica; Centre National de la Recherche Scientifique; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Ciencia, Tecnología e Innovación Productiva; Space Telescope Science Institute; Australian Research Council; Smithsonian Institution; National Science Foundation","keywords":"Cluster (spacecraft); Mass distribution; Observable; Galaxy cluster; Galaxy groups and clusters; Galaxy; Mass segregation; Brightest cluster galaxy","score_opus":0.013042736536213136,"score_gpt":0.21931529960600218,"score_spread":0.20627256306978906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1516723655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99831855,0.000037462367,0.00017852451,0.000018312909,0.0000025124107,0.0000048671577,0.000597649,0.00003423443,0.0008079083],"genre_scores_gemma":[0.9963445,0.00003201844,0.000662209,0.000015424583,0.000011333702,0.0000055322726,0.002114435,0.000022988414,0.0007915019],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998994,0.0000050662734,0.0000035428918,0.000033407443,0.000028250235,0.000030318688],"domain_scores_gemma":[0.99952745,0.000026459842,0.0001396692,0.000068785725,0.000103257444,0.000134378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014365629,0.00031762142,0.0002532148,0.0019837748,0.0005129789,0.00037967565,0.00047716565,0.00025269866,0.0013871309],"category_scores_gemma":[0.00030764597,0.00018194334,0.0003244037,0.001234043,0.00027712167,0.00020692124,0.0005050222,0.00022123723,0.0005711978],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034495225,0.00013386946,0.8977738,0.000036805293,0.00022433481,0.0010178868,0.0007610878,0.0015268149,0.07988459,0.00051429996,0.0026206747,0.015160952],"study_design_scores_gemma":[0.000005688968,0.000023588846,0.99474096,0.0000015853416,0.00002611276,0.00019292106,0.00018651265,0.001348875,0.00260707,0.00006638983,0.0007929411,0.0000073144483],"about_ca_topic_score_codex":0.025265237,"about_ca_topic_score_gemma":0.0491218,"teacher_disagreement_score":0.025265237,"about_ca_system_score_codex":0.0006640086,"about_ca_system_score_gemma":0.0002494113,"threshold_uncertainty_score":0.050236344},"labels":[],"label_agreement":null},{"id":"W1517437856","doi":"10.1088/0004-637x/745/2/161","title":"AN OPTICAL SURVEY FOR MILLIMETER-SIZED INTERSTELLAR METEOROIDS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Western University","funders":"","keywords":"Meteoroid; Meteor (satellite); Observatory; Limiting; Limiting magnitude; Meteorite; Planet; Flux (metallurgy)","score_opus":0.022116548785203798,"score_gpt":0.2629429100652205,"score_spread":0.24082636128001672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1517437856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98885906,0.0004542454,0.0005386746,0.000062109655,0.000012849265,0.00006462621,0.005656495,0.00008860152,0.0042634173],"genre_scores_gemma":[0.9832472,0.00053609774,0.0028742475,0.00009471516,0.000043485346,0.000044581066,0.00991265,0.000021593098,0.0032254544],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998148,0.000010892032,0.000010081151,0.000047800375,0.000079054356,0.00003734481],"domain_scores_gemma":[0.9991591,0.00003470326,0.000224832,0.00005471045,0.0002829896,0.00024364771],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002495842,0.0002543028,0.00011439018,0.0022942547,0.0005399954,0.00028300617,0.000348531,0.00013755714,0.0013342465],"category_scores_gemma":[0.00039641248,0.00012224521,0.00009557983,0.0013067232,0.000117418094,0.00028550733,0.00031573206,0.00016255418,0.0005239092],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008369896,0.000074430616,0.9465235,0.000058974103,0.00002720201,0.00016695684,0.0003753161,0.00007107857,0.016297378,0.000061565726,0.0027779315,0.03348194],"study_design_scores_gemma":[0.0000022827523,0.000038206726,0.9956435,0.0000036794124,0.0000049462114,0.00011416304,0.000102117876,0.00006929683,0.00039725093,0.0000059137797,0.0036165852,0.000002030343],"about_ca_topic_score_codex":0.067294665,"about_ca_topic_score_gemma":0.1547374,"teacher_disagreement_score":0.067294665,"about_ca_system_score_codex":0.00066095154,"about_ca_system_score_gemma":0.00064824626,"threshold_uncertainty_score":0.13380593},"labels":[],"label_agreement":null},{"id":"W1517919077","doi":"10.1088/0004-637x/806/1/133","title":"A GEMINI/GMOS STUDY OF INTERMEDIATE LUMINOSITY EARLY-TYPE VIRGO CLUSTER GALAXIES. I. GLOBULAR CLUSTER AND STELLAR KINEMATICS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Centro de Astrofísica y Tecnologías Afines; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Natural Science Foundation of China; Comisión Nacional de Investigación Científica y Tecnológica; Chinese Academy of Sciences; Agence Nationale de la Recherche; Institut Universitaire de France; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Virgo Cluster; Globular cluster; Galaxy; Stellar kinematics; Kinematics; Astronomy; Stars; Elliptical galaxy; Milky Way","score_opus":0.01729379400522811,"score_gpt":0.24115597707671602,"score_spread":0.22386218307148792,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1517919077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996425,0.00028563966,0.000077608594,0.00011398035,0.0000037276964,0.000004672552,0.00042077506,0.000010906166,0.0026577814],"genre_scores_gemma":[0.9972481,0.00017610859,0.0002325527,0.000031397456,0.000013702557,0.0000031191573,0.00073538587,0.000011734321,0.0015479145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998671,0.000026856287,0.000004907138,0.000031010728,0.000025015153,0.00004511961],"domain_scores_gemma":[0.99953187,0.000054746524,0.00010860372,0.000045621975,0.000059478047,0.00019979742],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004509982,0.0002283318,0.00019841072,0.002206934,0.0007288512,0.00081552216,0.00032411804,0.0002520752,0.00121895],"category_scores_gemma":[0.0005855974,0.00014759661,0.00023592856,0.0029092527,0.00037585883,0.00056088396,0.0007493715,0.00025930308,0.00042628954],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017575726,0.00012692237,0.97190225,0.000033695065,0.000049856146,0.00045737703,0.0027450712,0.0006026214,0.0033005583,0.003928782,0.0015051535,0.015171894],"study_design_scores_gemma":[0.0000023099299,0.00001854226,0.99574727,0.000005183769,0.0000092151595,0.00009006795,0.0012156462,0.00051116565,0.00013768714,0.00021198585,0.0020481562,0.0000027756987],"about_ca_topic_score_codex":0.060734626,"about_ca_topic_score_gemma":0.09327902,"teacher_disagreement_score":0.060734626,"about_ca_system_score_codex":0.001401495,"about_ca_system_score_gemma":0.00049042876,"threshold_uncertainty_score":0.12076223},"labels":[],"label_agreement":null},{"id":"W1518911068","doi":"10.1088/0004-637x/727/1/39","title":"ARE RADIO ACTIVE GALACTIC NUCLEI POWERED BY ACCRETION OR BLACK HOLE SPIN?","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Accretion (finance); Active galactic nucleus; Galaxy; Black hole (networking); Bulge; Supermassive black hole; Astronomy; Star formation","score_opus":0.007485457632438054,"score_gpt":0.22689585973909082,"score_spread":0.21941040210665277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1518911068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99822134,0.0003386669,0.00015138957,0.00005092302,0.000005346204,0.000003313041,0.00005288464,0.000007729491,0.0011683644],"genre_scores_gemma":[0.9996779,0.00008787093,0.000059918657,0.000020583608,0.000015995362,0.0000011215702,0.000042445517,0.0000019607974,0.00009219146],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997373,0.000050039107,0.0000167418,0.000056331133,0.000050106104,0.000089592955],"domain_scores_gemma":[0.99725693,0.00078986504,0.0012852985,0.00017703985,0.00013520833,0.0003557146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006789374,0.0002878985,0.00033976696,0.00087174977,0.00020818778,0.0013643133,0.0004130906,0.00048190157,0.0015621857],"category_scores_gemma":[0.0034398376,0.00014791489,0.00025384617,0.0003862482,0.00079654664,0.00082357443,0.00049041846,0.00023503945,0.00040886743],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034538205,0.000047195186,0.9841353,0.000027076288,0.00008493829,0.00039518607,0.00018954961,0.0002438691,0.006228981,0.00042458315,0.00008652398,0.0077912444],"study_design_scores_gemma":[0.000014961833,0.00012213619,0.9958566,0.000010054005,0.000060223836,0.0005795767,0.0003396793,0.0012549002,0.000862491,0.0006064877,0.00028575098,0.000007169598],"about_ca_topic_score_codex":0.0011094068,"about_ca_topic_score_gemma":0.0013211521,"teacher_disagreement_score":0.0015621857,"about_ca_system_score_codex":0.000258002,"about_ca_system_score_gemma":0.0001035769,"threshold_uncertainty_score":0.005226016},"labels":[],"label_agreement":null},{"id":"W1520813977","doi":"10.1088/0004-637x/722/2/1325","title":"CONFRONTING THREE-DIMENSIONAL TIME-DEPENDENT JET SIMULATIONS WITH<i>HUBBLE SPACE TELESCOPE</i>OBSERVATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Calgary","funders":"","keywords":"Jet (fluid); Computational astrophysics; Rotation (mathematics); Line (geometry); Magnetic field; Space (punctuation); Field (mathematics)","score_opus":0.01141374090927784,"score_gpt":0.22680799336638668,"score_spread":0.21539425245710883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1520813977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97938675,0.00020506057,0.009641534,0.00041851625,0.00007857997,0.000068793604,0.001724684,0.00038516862,0.008090967],"genre_scores_gemma":[0.99017966,0.00014784955,0.006952006,0.00014696982,0.000036782913,0.00008812887,0.0015051186,0.0001024334,0.00084099424],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99974257,0.00005650942,0.000016948316,0.00005126013,0.000054964203,0.00007779336],"domain_scores_gemma":[0.9966011,0.0023715193,0.0002804114,0.00016939953,0.0002848525,0.000292714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055179663,0.00073446543,0.0008539931,0.00073281757,0.00085206755,0.0013650878,0.0017500218,0.0019529159,0.0030688331],"category_scores_gemma":[0.0040855776,0.0006713683,0.00094879343,0.00089008466,0.0010147,0.0006737097,0.00071723515,0.0016745062,0.00027119342],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008886897,0.00006754228,0.0032195912,0.000022377319,0.000044054083,0.00008919135,0.000050598795,0.99441165,0.0004900533,0.00066869607,0.00020793399,0.00063946436],"study_design_scores_gemma":[0.000044348773,0.00002736807,0.0010941635,0.000004402524,0.00001246745,0.00001435753,0.000027816426,0.99799514,0.00030858515,0.00027409694,0.00018798621,0.000009245621],"about_ca_topic_score_codex":0.044589665,"about_ca_topic_score_gemma":0.024708144,"teacher_disagreement_score":0.044589665,"about_ca_system_score_codex":0.001606397,"about_ca_system_score_gemma":0.0011167588,"threshold_uncertainty_score":0.08866024},"labels":[],"label_agreement":null},{"id":"W1520858193","doi":"10.1086/341545","title":"The Distance to Supernova Remnant CTB 109 Deduced from Its Environment","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Supernova remnant; Spiral galaxy; Galactic plane; Spiral (railway); Supernova; H II region; Enhanced Data Rates for GSM Evolution","score_opus":0.011507536313013286,"score_gpt":0.2000552331031625,"score_spread":0.1885476967901492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1520858193","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996696,0.00019138082,0.00028415082,0.000014227661,0.000004733966,0.000005299768,0.00043119123,0.000022006348,0.002351045],"genre_scores_gemma":[0.99826056,0.00009914823,0.000333598,0.000005190395,0.000004140512,0.0000034903803,0.0010950897,0.000005958461,0.00019280896],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999899,0.000009171524,0.000007481283,0.00004024045,0.000026311372,0.000017697164],"domain_scores_gemma":[0.9994709,0.000071355964,0.00014940635,0.000052580275,0.00009463123,0.00016117666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012024707,0.00020851754,0.0003074047,0.00080158276,0.00036019148,0.0004546454,0.00027328698,0.00021039361,0.0012613691],"category_scores_gemma":[0.0009911295,0.00014530687,0.00016606158,0.0006446212,0.00028319538,0.00025622814,0.000599763,0.00031699098,0.00055306824],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008059895,0.00005696963,0.86029226,0.00012875973,0.000119677345,0.0023592268,0.00025700187,0.00600445,0.11856239,0.0015809444,0.0006475881,0.009184767],"study_design_scores_gemma":[0.000011294518,0.0001248604,0.9883067,0.00000913848,0.000032327705,0.0011210318,0.00014925444,0.0026070212,0.005921803,0.00024818315,0.0014512626,0.000017080794],"about_ca_topic_score_codex":0.0062597,"about_ca_topic_score_gemma":0.0035796713,"teacher_disagreement_score":0.0062597,"about_ca_system_score_codex":0.00048032904,"about_ca_system_score_gemma":0.00020553537,"threshold_uncertainty_score":0.012446523},"labels":[],"label_agreement":null},{"id":"W1520907587","doi":"10.1088/0004-637x/808/1/88","title":"<i>HST</i>/STIS ULTRAVIOLET SPECTROSCOPY OF THE COMPONENTS OF THE MASSIVE TRIPLE STAR<i>δ</i>ORI A","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":197,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"Stars; Spectral line; Spectroscopy; Ultraviolet; Flux (metallurgy); Ultraviolet astronomy; Component (thermodynamics); Star (game theory)","score_opus":0.0158313968084771,"score_gpt":0.24052038914473117,"score_spread":0.22468899233625408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1520907587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9815626,0.00036796398,0.0024125695,0.00010982603,0.00004380313,0.000025851687,0.004451012,0.0005080256,0.010518372],"genre_scores_gemma":[0.9846139,0.0002289636,0.0090757795,0.000084128566,0.000051802974,0.000013543869,0.0044754916,0.00007874911,0.0013776809],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.0000059957338,0.000006502017,0.00001783905,0.000030245625,0.000010401258],"domain_scores_gemma":[0.9996722,0.000022724997,0.00010895657,0.000044603756,0.0000681075,0.00008342573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019521273,0.0002855868,0.0001513366,0.0018482289,0.00043242078,0.0004142474,0.00024438306,0.00022554513,0.0025013254],"category_scores_gemma":[0.0002783118,0.00014241447,0.00018672415,0.0012344251,0.00015500527,0.0002986242,0.00035070346,0.00033590526,0.00045630825],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041806916,0.0002980669,0.4469638,0.0002673853,0.00020490763,0.0018344475,0.0008815283,0.0016382366,0.47509134,0.0015024862,0.011027702,0.05987208],"study_design_scores_gemma":[0.000009480206,0.00012838046,0.9628624,0.000025333406,0.00005262662,0.0012862525,0.00023316614,0.0032981003,0.0234449,0.00037385346,0.008264952,0.000020583464],"about_ca_topic_score_codex":0.0021945366,"about_ca_topic_score_gemma":0.004389389,"teacher_disagreement_score":0.0025013254,"about_ca_system_score_codex":0.0001555448,"about_ca_system_score_gemma":0.00013295011,"threshold_uncertainty_score":0.0083678365},"labels":[],"label_agreement":null},{"id":"W1525297841","doi":"10.1088/0004-637x/811/1/42","title":"THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: ENSEMBLE SPECTROSCOPIC VARIABILITY OF QUASAR BROAD EMISSION LINES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Quasar; Reverberation mapping; Physics; Astrophysics; Sky; Emission spectrum; Rest frame; Astronomy; Spectral line; Galaxy; Redshift","score_opus":0.020985041493288524,"score_gpt":0.2509109380642819,"score_spread":0.22992589657099335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1525297841","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22108673,0.0011913871,0.0077685793,0.0060622897,0.0007592569,0.00034622406,0.73958343,0.0020414006,0.021160716],"genre_scores_gemma":[0.38848364,0.00064778735,0.014650054,0.0004093133,0.00032410302,0.0002601379,0.584275,0.0007588324,0.010191127],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9985846,0.00040546554,0.000053143372,0.00019299648,0.00050188205,0.00026201026],"domain_scores_gemma":[0.9956713,0.00025166792,0.0005759988,0.0007503137,0.0012473783,0.0015034314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0033650673,0.000992035,0.00087471015,0.0032639927,0.000816703,0.0008270713,0.0016987304,0.0003597087,0.0051476364],"category_scores_gemma":[0.0025729428,0.0002884565,0.0005416091,0.0039262963,0.0002835604,0.0012567539,0.002311246,0.0010990609,0.00264347],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012480685,0.0006159209,0.20962709,0.00020554094,0.0005821964,0.0003654114,0.0008936363,0.002408131,0.0065763923,0.004679532,0.6344197,0.13837843],"study_design_scores_gemma":[0.00030928335,0.0001369152,0.8439753,0.000047535716,0.00010412999,0.00011994709,0.00041926847,0.006786487,0.0026695984,0.0023077948,0.14303744,0.000086393506],"about_ca_topic_score_codex":0.07713753,"about_ca_topic_score_gemma":0.09643339,"teacher_disagreement_score":0.07713753,"about_ca_system_score_codex":0.0014068345,"about_ca_system_score_gemma":0.0031565859,"threshold_uncertainty_score":0.15337706},"labels":[],"label_agreement":null},{"id":"W1526857352","doi":"10.1086/510061","title":"Deep Submillimeter Observations of Two Lyα‐emitting Galaxies at<i>z</i>∼ 6.5","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Galaxy; Astrophysics; Confusion; Star formation; Astronomy; Population; Hubble Deep Field; Submillimeter wave; Redshift; Millimeter","score_opus":0.014465177035789421,"score_gpt":0.231590726579908,"score_spread":0.21712554954411858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1526857352","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977574,0.00007870945,0.00055530824,0.00003064325,0.0000045661027,0.000008765459,0.00017140548,0.000040121646,0.0013531465],"genre_scores_gemma":[0.99710137,0.000051108913,0.0016082701,0.00006138078,0.000016814949,0.000010118352,0.00060117384,0.0000054520224,0.00054444186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998957,0.0000060183806,0.0000040645964,0.000023151435,0.000022383698,0.000048662652],"domain_scores_gemma":[0.99953866,0.000048933474,0.00012579896,0.00004028253,0.000035497542,0.00021077291],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024247893,0.0002230673,0.00022093451,0.0009040797,0.00036657994,0.00037308253,0.00030600143,0.00036843578,0.0009049515],"category_scores_gemma":[0.0003483853,0.0002874087,0.0001577264,0.00036682643,0.00019184352,0.00026132507,0.00056526467,0.0003922805,0.00031305154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005358157,0.0004020251,0.776615,0.000054707063,0.00009333449,0.00080237724,0.0015618346,0.00036210634,0.1786831,0.0006698706,0.0010212918,0.03919849],"study_design_scores_gemma":[0.00001512363,0.00009853187,0.9961951,0.00000459755,0.000014455007,0.00024880693,0.00011061039,0.000276805,0.0018136046,0.000093807415,0.001123433,0.0000051606826],"about_ca_topic_score_codex":0.0018702648,"about_ca_topic_score_gemma":0.004748892,"teacher_disagreement_score":0.0018702648,"about_ca_system_score_codex":0.0002282271,"about_ca_system_score_gemma":0.000074615906,"threshold_uncertainty_score":0.0037187934},"labels":[],"label_agreement":null},{"id":"W1527102485","doi":"10.1086/339233","title":"Black Hole Growth in Dark Matter and the<i>M</i><sub>BH</sub>‐σ Relation","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Dark matter; Black hole (networking); Velocity dispersion; Adiabatic process; Primordial black hole; Dark matter halo; Power law; Halo; Galaxy; Spin-flip; Quantum mechanics; Statistics","score_opus":0.00543885818216035,"score_gpt":0.17944292372885787,"score_spread":0.1740040655466975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1527102485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9901922,0.00032017176,0.004704123,0.0000707547,0.0000025393551,0.000004561329,0.000018720346,0.000028919301,0.0046580923],"genre_scores_gemma":[0.99881387,0.000111340945,0.00074863853,0.000005426203,0.0000032057246,0.000002552694,0.0000116061865,0.000004145874,0.00029923074],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995196,0.000011756612,0.0000026563498,0.000007632881,0.000011450315,0.0000145566155],"domain_scores_gemma":[0.9989863,0.00046004355,0.000312418,0.000080439386,0.00008641646,0.00007436305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022612995,0.00017469435,0.00008511341,0.0003932984,0.00021465716,0.00039383344,0.00017049733,0.00018946468,0.00094748504],"category_scores_gemma":[0.00247327,0.00010879655,0.00015100508,0.00021917773,0.0007458971,0.00056151696,0.00043257725,0.00020564532,0.00013606877],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048344,0.00008476149,0.40755555,0.00017483608,0.000075337244,0.0020822526,0.0011663616,0.13442539,0.11534044,0.28128794,0.0007314496,0.05659226],"study_design_scores_gemma":[0.000051162864,0.00021559115,0.3800594,0.000043513057,0.00005543844,0.0027132048,0.00064708095,0.3579837,0.0731995,0.1814704,0.00350742,0.000053591233],"about_ca_topic_score_codex":0.0014945214,"about_ca_topic_score_gemma":0.00090297515,"teacher_disagreement_score":0.0014945214,"about_ca_system_score_codex":0.00045971284,"about_ca_system_score_gemma":0.0001549444,"threshold_uncertainty_score":0.003335476},"labels":[],"label_agreement":null},{"id":"W1527733219","doi":"10.3847/0004-637x/818/2/159","title":"DETECTION AND CHARACTERIZATION OF EXTRASOLAR PLANETS THROUGH MEAN-MOTION RESONANCES. I. SIMULATIONS OF HYPOTHETICAL DEBRIS DISKS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Planet; Exoplanet; Debris disk; Planetary system; Eccentricity (behavior); Debris; Planetary mass; Orbit (dynamics)","score_opus":0.013317526750192897,"score_gpt":0.23333027241846024,"score_spread":0.22001274566826734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1527733219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99580574,0.000054790333,0.0023166381,0.0000899155,0.000007882118,0.0000137997495,0.00014669212,0.000051738578,0.0015128233],"genre_scores_gemma":[0.99875677,0.000013983109,0.0009872459,0.000010951461,0.0000021081883,0.000007393675,0.00007320689,0.00000940319,0.00013881974],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989283,0.000030519095,0.000005824937,0.000020516825,0.000017714376,0.000032469932],"domain_scores_gemma":[0.9987476,0.00069359416,0.00015163413,0.00012780023,0.00007879222,0.00020051857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004904958,0.00028678245,0.00045202553,0.00043379358,0.00059476384,0.0006042813,0.00077500904,0.0007800068,0.0011583152],"category_scores_gemma":[0.0026439354,0.00027944316,0.0005794708,0.00024380613,0.00083360955,0.00065043545,0.0007307025,0.0006392155,0.000095223404],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026885857,0.00012175028,0.027006304,0.00004376903,0.00007749198,0.0002307611,0.00018185236,0.9626301,0.0048025534,0.0026690764,0.00030100506,0.0016664524],"study_design_scores_gemma":[0.000040470197,0.000058655845,0.0036166455,0.0000039342567,0.000010171786,0.000026199592,0.00005046637,0.9946792,0.00059050135,0.00076046697,0.00015608553,0.0000072275566],"about_ca_topic_score_codex":0.0077701323,"about_ca_topic_score_gemma":0.004773793,"teacher_disagreement_score":0.0077701323,"about_ca_system_score_codex":0.00064857904,"about_ca_system_score_gemma":0.0003632729,"threshold_uncertainty_score":0.015449762},"labels":[],"label_agreement":null},{"id":"W1535066424","doi":"10.3847/0004-637x/819/1/21","title":"DIFFUSE CORONAE IN COSMOLOGICAL SIMULATIONS OF MILKY WAY-SIZED GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Halo; Virial mass; Galaxy; Virial theorem; Baryon; Galactic halo; Luminosity; Galaxy formation and evolution","score_opus":0.01231204391750908,"score_gpt":0.22851646585508026,"score_spread":0.21620442193757117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1535066424","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985507,0.00003690971,0.00044775516,0.00007007706,0.000005651377,0.000007988453,0.00013387235,0.00006487005,0.00068222894],"genre_scores_gemma":[0.99790597,0.00004056766,0.0014010447,0.00004435534,0.0000066591692,0.000014307686,0.00031226623,0.000028126964,0.00024672295],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987483,0.000045697514,0.0000060366087,0.00002571478,0.000018145345,0.000029568473],"domain_scores_gemma":[0.9989672,0.0004951892,0.000112377624,0.00008814491,0.00010472768,0.00023238642],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059025345,0.0004322695,0.00045896586,0.00053239975,0.0005130111,0.00078943704,0.0016472467,0.00094161957,0.0016634269],"category_scores_gemma":[0.0022224393,0.000345429,0.0007536124,0.0005472567,0.00068687677,0.00052435714,0.0007844028,0.00075495726,0.00014237958],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036335847,0.0003343389,0.041315004,0.000045155255,0.00020440048,0.00024279223,0.0002544351,0.95036846,0.0025485,0.0018079208,0.00048948184,0.0020262084],"study_design_scores_gemma":[0.00014412131,0.00013430355,0.008514315,0.0000073536744,0.00003704156,0.000026638847,0.00011612367,0.9897827,0.0004892725,0.00039185875,0.00034238264,0.000013888452],"about_ca_topic_score_codex":0.03905761,"about_ca_topic_score_gemma":0.023694417,"teacher_disagreement_score":0.03905761,"about_ca_system_score_codex":0.0014603225,"about_ca_system_score_gemma":0.00059250265,"threshold_uncertainty_score":0.07766056},"labels":[],"label_agreement":null},{"id":"W1535564063","doi":"10.1088/0004-637x/752/1/69","title":"THE BORON-TO-CARBON ABUNDANCE RATIO AND GALACTIC PROPAGATION OF COSMIC RADIATION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radiation Therapy and Dosimetry","field":"Medicine","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Stichting voor Fundamenteel Onderzoek der Materie; National Aeronautics and Space Administration","keywords":"Cosmic ray; Physics; Astrophysics; Lambda; Exponent; Power law; Natural abundance; Galaxy; Isotopes of boron; Path length; Spectral line; Energy (signal processing); Attenuation length; Computational physics; Boron; Nuclear physics; Astronomy; Optics; Statistics; Isotope","score_opus":0.008256689423158632,"score_gpt":0.25683500590545627,"score_spread":0.24857831648229764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1535564063","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97648686,0.0076258164,0.0027007635,0.00027386035,0.000040844454,0.00000998568,0.0023039088,0.00016614526,0.010391798],"genre_scores_gemma":[0.9964551,0.0009823815,0.0005307768,0.000028338925,0.000017432436,0.0000025351192,0.0006454648,0.000038611277,0.0012993774],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999884,0.00002970288,0.000010460246,0.00003275222,0.000026577922,0.000016455915],"domain_scores_gemma":[0.9993874,0.00018431905,0.00020541559,0.000032327243,0.0001090071,0.00008158697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002570361,0.00017622147,0.00017513901,0.0010874124,0.00011121287,0.00062828953,0.00020948304,0.00046603286,0.004035604],"category_scores_gemma":[0.001195692,0.00019437693,0.00014609893,0.0007350421,0.0001518861,0.00038548274,0.00016695815,0.000251719,0.0010977455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00667874,0.00009794668,0.7105931,0.00039799174,0.00054378744,0.0011255239,0.00033798613,0.0030512018,0.17219475,0.0036291892,0.0030201036,0.09832963],"study_design_scores_gemma":[0.00004748546,0.0003584013,0.95121455,0.000054721357,0.00024794688,0.0036947734,0.00024366859,0.0029588137,0.03630484,0.0012663346,0.0035598818,0.00004857952],"about_ca_topic_score_codex":0.0030363968,"about_ca_topic_score_gemma":0.0021958067,"teacher_disagreement_score":0.004035604,"about_ca_system_score_codex":0.0003295417,"about_ca_system_score_gemma":0.00015013904,"threshold_uncertainty_score":0.013500392},"labels":[],"label_agreement":null},{"id":"W1537085661","doi":"10.1086/343077","title":"<i>Submillimeter Wave Astronomy Satellite</i>and Arecibo Observations of H<sub>2</sub>O and OH in a Diffuse Cloud along the Line of Sight to W51","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Line-of-sight; Molecular cloud; Line (geometry); Ultraviolet; Water vapor; Telescope; Satellite; Absorption (acoustics); Radio telescope","score_opus":0.02430415832937629,"score_gpt":0.21502420741512748,"score_spread":0.1907200490857512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1537085661","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97665113,0.00088134786,0.0007815555,0.00022649937,0.000041149393,0.000045083263,0.0036311026,0.00007156706,0.017670702],"genre_scores_gemma":[0.97954684,0.00070844154,0.0030481813,0.00015467028,0.00006736481,0.000024645946,0.011353348,0.000018044191,0.0050784955],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999112,0.000004207723,0.000003907279,0.000017830329,0.00003497721,0.000027950906],"domain_scores_gemma":[0.9996761,0.000016901062,0.00015588092,0.000034862962,0.000046233337,0.000070066046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015295287,0.00021052928,0.00011636965,0.00077368197,0.00030234177,0.00036575788,0.00020770934,0.00016506844,0.0025772967],"category_scores_gemma":[0.0002425483,0.0001286397,0.00014471865,0.000702644,0.00017195003,0.00038009067,0.0004358933,0.00020602942,0.0005354877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003933254,0.00011602421,0.7909253,0.00021205936,0.00016369169,0.00047671743,0.00048921676,0.0003674075,0.106727794,0.0014063533,0.0073000323,0.09142201],"study_design_scores_gemma":[0.000007881736,0.000020559215,0.9920797,0.000007724757,0.000009242484,0.00007351383,0.00005380136,0.00010882943,0.0015669436,0.000076148695,0.0059933728,0.000002328435],"about_ca_topic_score_codex":0.0098703485,"about_ca_topic_score_gemma":0.043459017,"teacher_disagreement_score":0.0098703485,"about_ca_system_score_codex":0.00028908838,"about_ca_system_score_gemma":0.00017290526,"threshold_uncertainty_score":0.019625783},"labels":[],"label_agreement":null},{"id":"W1537744696","doi":"10.1086/320571","title":"Evidence for a Sudden Magnetic Field Reconfiguration in Soft Gamma Repeater 1900+14","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Flare; Flux (metallurgy); Astrophysics; Physics; Pulse (music); Gamma ray; Magnetic flux; Repeater (horology); Magnetic field; Neutron star; Solar flare; Optics; Chemistry; Detector; Materials science","score_opus":0.03734560059727246,"score_gpt":0.3473902044554614,"score_spread":0.310044603858189,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1537744696","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994363,0.000036046258,0.000067480076,0.000013266635,0.0000025943061,0.0000030455437,0.00007481263,0.00001348782,0.00035288147],"genre_scores_gemma":[0.99876726,0.000048986538,0.00027310487,0.00003651448,0.000013742303,0.0000075098365,0.00057141687,0.000006718165,0.00027482328],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994123,0.000004640807,0.000003139744,0.000015731062,0.0000132243895,0.000022059543],"domain_scores_gemma":[0.99960405,0.000026887608,0.0002031943,0.000031323176,0.000052334326,0.0000822236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012086532,0.00015587948,0.00027127718,0.00051974907,0.0002704949,0.00028799704,0.00029717118,0.00030711116,0.000860057],"category_scores_gemma":[0.00038609747,0.00013736643,0.00013535212,0.00031803956,0.000389813,0.00011452749,0.00035725697,0.00033476079,0.00024630892],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079006644,0.00012963131,0.7268304,0.0000629105,0.00007541236,0.0012800744,0.00052712654,0.00025509595,0.25778916,0.00018450122,0.00056742993,0.011508169],"study_design_scores_gemma":[0.000010331919,0.00021747366,0.9951574,0.0000026009454,0.000013183534,0.00057124376,0.000077872624,0.00014635161,0.0032744308,0.000036112564,0.0004883927,0.000004616782],"about_ca_topic_score_codex":0.0024321273,"about_ca_topic_score_gemma":0.004132834,"teacher_disagreement_score":0.0024321273,"about_ca_system_score_codex":0.0002500327,"about_ca_system_score_gemma":0.00012773165,"threshold_uncertainty_score":0.0048359036},"labels":[],"label_agreement":null},{"id":"W1543909229","doi":"10.1086/379281","title":"A Planetary Companion to γ Cephei A","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":332,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia","funders":"","keywords":"Radial velocity; Physics; Orbital period; Astrophysics; Photometry (optics); Planet; Amplitude; Exoplanet; Orbit (dynamics); Residual; Orbital inclination; Astronomy; Binary number; Stars; Mathematics","score_opus":0.01186486263041416,"score_gpt":0.2202459427015059,"score_spread":0.20838108007109174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1543909229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99163276,0.0005723426,0.0006916581,0.00010791266,0.00006865445,0.00001920881,0.00016828293,0.00003484924,0.0067043235],"genre_scores_gemma":[0.9982326,0.00015062199,0.0004257598,0.00008676723,0.000035939967,0.000005398169,0.00023875796,0.0000047049193,0.00081944757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984205,0.000007719635,0.000009132703,0.00006348227,0.000038982384,0.000038569655],"domain_scores_gemma":[0.9994955,0.00009124128,0.00017177254,0.000091216745,0.000051623647,0.000098629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017372164,0.0002597502,0.00021780301,0.0006115096,0.0012586088,0.0009900498,0.00034648806,0.00042797686,0.0026875662],"category_scores_gemma":[0.00095210236,0.00016662339,0.000111186455,0.00054031383,0.0005367499,0.0003838443,0.00084159157,0.000511774,0.00085169985],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006230184,0.00025305458,0.8013056,0.00016636973,0.00007386225,0.022900824,0.0029258882,0.00028394768,0.08574992,0.004850146,0.0049676625,0.07589979],"study_design_scores_gemma":[0.000047736623,0.0015760704,0.84909725,0.000058419344,0.00009554387,0.074582756,0.0011504905,0.00093949196,0.0127169285,0.0024504596,0.057231173,0.000053703883],"about_ca_topic_score_codex":0.0022049127,"about_ca_topic_score_gemma":0.0016719264,"teacher_disagreement_score":0.0026875662,"about_ca_system_score_codex":0.00018224127,"about_ca_system_score_gemma":0.00020003825,"threshold_uncertainty_score":0.008990824},"labels":[],"label_agreement":null},{"id":"W1545521998","doi":"10.1088/0004-637x/806/1/140","title":"<i>Einstein@Home</i>DISCOVERY OF A PALFA MILLISECOND PULSAR IN AN ECCENTRIC BINARY ORBIT","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Office of Naval Research; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Max-Planck-Gesellschaft; Canada Research Chairs; Canadian Institute for Advanced Research; Fonds Québécois de la Recherche sur la Nature et les Technologies; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Science Foundation","keywords":"Millisecond pulsar; White dwarf; Neutron star; Pulsar; Orbit (dynamics); Circumbinary planet; Binary number; Binary pulsar; Binary star; Proper motion","score_opus":0.019870454719097656,"score_gpt":0.30685222386426253,"score_spread":0.2869817691451649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1545521998","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.09302092,0.026765762,0.012683123,0.14293209,0.041682463,0.00078300847,0.10165033,0.009151154,0.5713312],"genre_scores_gemma":[0.4435532,0.022790587,0.03216464,0.027185231,0.036876976,0.00043751978,0.09067474,0.0032760906,0.34304103],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99911755,0.00009272908,0.00008442298,0.0001357169,0.0005056672,0.00006380785],"domain_scores_gemma":[0.99566025,0.0011258096,0.00091978884,0.0008275874,0.000822827,0.0006437627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025521854,0.00034632607,0.00040398343,0.0038529981,0.0010198681,0.0017836484,0.00047572618,0.0009743065,0.0306068],"category_scores_gemma":[0.006763351,0.00020646203,0.00035285583,0.0032286076,0.00065553666,0.0008520485,0.0016112614,0.0007994773,0.011896348],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040076344,0.00004133981,0.022337064,0.0003979907,0.00007943873,0.001279527,0.00033369445,0.00007475514,0.0058669713,0.006687706,0.8875989,0.07490181],"study_design_scores_gemma":[0.000038856175,0.0000934297,0.07787255,0.00022366071,0.000040207993,0.0019788707,0.00017453267,0.00016281955,0.0054134363,0.0020868885,0.9118816,0.00003305092],"about_ca_topic_score_codex":0.0027684316,"about_ca_topic_score_gemma":0.0071205017,"teacher_disagreement_score":0.0306068,"about_ca_system_score_codex":0.00093282975,"about_ca_system_score_gemma":0.0009140875,"threshold_uncertainty_score":0.10238999},"labels":[],"label_agreement":null},{"id":"W1545748505","doi":"10.1088/0004-637x/805/1/30","title":"SUB-mm JET PROPERTIES OF THE X-RAY BINARY SWIFT J1745–26","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Alberta","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; National Science Foundation; Ministerio de Economía y Competitividad; Smithsonian Institution; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Academia Sinica","keywords":"Spectral index; Jet (fluid); Accretion (finance); Spectral line; Spectral analysis; Accretion disc; Binary number; Astrophysical jet; Radio spectrum; X-ray binary","score_opus":0.029438596663326475,"score_gpt":0.22527406649708673,"score_spread":0.19583546983376027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1545748505","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984555,0.00015139434,0.00022849202,0.000018166842,0.0000066613757,0.000002965121,0.00028370984,0.000027374143,0.00082579517],"genre_scores_gemma":[0.998116,0.00007233102,0.00044356976,0.000020575451,0.000018474753,0.00000613926,0.0009041939,0.000019459465,0.00039934932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995434,0.0000020772632,0.000002525546,0.000014565454,0.000012075831,0.000014466074],"domain_scores_gemma":[0.99980944,0.000025413532,0.000089524765,0.000011987789,0.000020432735,0.000043282347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011723137,0.00024343145,0.00018935652,0.00072413916,0.0002570508,0.00045180175,0.00017243144,0.00017956666,0.0015084672],"category_scores_gemma":[0.00023887104,0.00015308315,0.00013963328,0.0004899797,0.00014490589,0.00022628954,0.0003497552,0.0002776024,0.00032608304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011024334,0.0001930969,0.67763495,0.000108083615,0.00013940915,0.001677659,0.0004973326,0.0017530433,0.28393218,0.0008136936,0.0016076615,0.030540353],"study_design_scores_gemma":[0.000014905854,0.000088496505,0.9922546,0.000005804736,0.000019896632,0.0002912787,0.0000736893,0.001373871,0.004814602,0.00008775876,0.00096760184,0.0000075187954],"about_ca_topic_score_codex":0.0013240282,"about_ca_topic_score_gemma":0.0026981875,"teacher_disagreement_score":0.0015084672,"about_ca_system_score_codex":0.00018348884,"about_ca_system_score_gemma":0.000057281195,"threshold_uncertainty_score":0.0050463676},"labels":[],"label_agreement":null},{"id":"W1546292687","doi":"10.1086/312592","title":"The Galactic Worm GW 123.4−1.5: A Mushroom-shaped H [CLC][CSC]i[/CSC][/CLC] Cloud","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto; Western University; Université de Montréal; University of Calgary; Queen's University","funders":"","keywords":"Physics; Galactic plane; Astrophysics; Telescope; HERA; Observatory; Astronomy; Stars; Particle physics","score_opus":0.008979583689826758,"score_gpt":0.23412018063293993,"score_spread":0.22514059694311317,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1546292687","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9918132,0.00004426171,0.002745641,0.00010963376,0.000012388059,0.000024710554,0.00014928658,0.00006274118,0.00503817],"genre_scores_gemma":[0.9979527,0.000028448101,0.001073168,0.000028105409,0.0000032232585,0.0000055180717,0.00014944996,0.000017149994,0.000742182],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99997604,0.0000024613003,5.677843e-7,0.000004047535,0.000004259524,0.000012569023],"domain_scores_gemma":[0.99993026,0.0000087606195,0.000011092949,0.000006601251,0.000004618738,0.00003862309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006968419,0.00023224088,0.0001697165,0.00015511677,0.00039581698,0.00046716325,0.00046708222,0.00034385273,0.0015440168],"category_scores_gemma":[0.0001824247,0.00013027793,0.00028770644,0.00011874289,0.00046083712,0.00033452758,0.00036498145,0.0003039235,0.00016649188],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012888159,0.00035833524,0.14567648,0.000117268646,0.00018044589,0.0066460567,0.00048076955,0.67795765,0.080527075,0.06260537,0.0074166167,0.01674506],"study_design_scores_gemma":[0.00029410233,0.00023517171,0.080368906,0.000018173449,0.00004973614,0.0010101793,0.00031926666,0.8978645,0.006159331,0.008804915,0.004832606,0.00004310926],"about_ca_topic_score_codex":0.013911456,"about_ca_topic_score_gemma":0.012640585,"teacher_disagreement_score":0.013911456,"about_ca_system_score_codex":0.0006151062,"about_ca_system_score_gemma":0.00034307444,"threshold_uncertainty_score":0.027660966},"labels":[],"label_agreement":null},{"id":"W1546338243","doi":"10.1086/345981","title":"The Cluster Mass Function from Early Sloan Digital Sky Survey Data: Cosmological Implications","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Sky; Physics; Cluster (spacecraft); Normalization (sociology); Astrophysics; Redshift; Galaxy; Amplitude; Galaxy cluster; Degeneracy (biology); Magnitude (astronomy); Optics","score_opus":0.02162401023499921,"score_gpt":0.23043883230562281,"score_spread":0.2088148220706236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1546338243","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98889554,0.00038600608,0.0043837675,0.00046549193,0.000011232673,0.000010575009,0.0017218482,0.000109164874,0.004016373],"genre_scores_gemma":[0.99569523,0.00012839264,0.0021099409,0.000034131906,0.0000092485025,0.000008342109,0.001582046,0.000035979374,0.00039658567],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997166,0.000117438234,0.000013722661,0.000053243613,0.00006710038,0.000031905838],"domain_scores_gemma":[0.9979673,0.0009810367,0.0003120431,0.00023586639,0.000288101,0.00021559358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001291556,0.00031424017,0.00023726738,0.0014025492,0.0004693788,0.0005667655,0.00061238615,0.00021945774,0.0017871761],"category_scores_gemma":[0.00526607,0.00012327709,0.00018646849,0.001458654,0.00034655313,0.00040153402,0.00044147318,0.00034778003,0.000312897],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031980695,0.000060326456,0.9003133,0.00015009234,0.00017836675,0.0004935603,0.00033503113,0.039160352,0.0055070007,0.017649077,0.0070551103,0.028777823],"study_design_scores_gemma":[0.000030188883,0.00002727359,0.8937041,0.000043704364,0.00005460118,0.00027157326,0.00030578507,0.088110566,0.0029429705,0.010636815,0.003820715,0.00005161255],"about_ca_topic_score_codex":0.046583824,"about_ca_topic_score_gemma":0.0368355,"teacher_disagreement_score":0.046583824,"about_ca_system_score_codex":0.0010564529,"about_ca_system_score_gemma":0.00066252885,"threshold_uncertainty_score":0.09262538},"labels":[],"label_agreement":null},{"id":"W1547430321","doi":"10.1088/0004-637x/808/1/91","title":"MEASURING INFRARED SURFACE BRIGHTNESS FLUCTUATION DISTANCES WITH<i>HST</i>WFC3: CALIBRATION AND ADVICE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Wide Field Camera 3; Astrophysics; Galaxy; Surface brightness; Surface brightness fluctuation; Luminosity; Infrared; Astronomy; Stellar population; Luminous infrared galaxy; Brightness; Calibration; Hubble space telescope; Lenticular galaxy; Star formation","score_opus":0.012837451544424531,"score_gpt":0.20141255960797771,"score_spread":0.18857510806355318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1547430321","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.64995974,0.00070662505,0.30428842,0.0002054534,0.000109154724,0.00016544391,0.02005018,0.010098401,0.01441663],"genre_scores_gemma":[0.7832086,0.00035343153,0.19158193,0.00014862485,0.0000697262,0.0001964417,0.0202385,0.0014156033,0.002787127],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99934775,0.00005577329,0.000041993666,0.00014153887,0.00034705325,0.0000660148],"domain_scores_gemma":[0.9983461,0.00013335641,0.00035038037,0.00051029125,0.0005552068,0.00010466077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010250014,0.00047006292,0.00027741428,0.0017239755,0.0002980542,0.000498267,0.0006562183,0.00025357306,0.001811542],"category_scores_gemma":[0.0018977706,0.00023237844,0.0003455784,0.0018532315,0.00021231167,0.0005932149,0.00044181946,0.00044667564,0.0013457917],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033920354,0.00010870191,0.5592477,0.0001208181,0.0001586023,0.00012628584,0.0004258487,0.008261522,0.093757495,0.0020987513,0.020078152,0.31527695],"study_design_scores_gemma":[0.000014538644,0.000034786175,0.89261866,0.000017908573,0.000038747607,0.00023974045,0.00008432238,0.03184649,0.057715967,0.0010387105,0.016277462,0.00007261436],"about_ca_topic_score_codex":0.02057395,"about_ca_topic_score_gemma":0.03307054,"teacher_disagreement_score":0.02057395,"about_ca_system_score_codex":0.0007076386,"about_ca_system_score_gemma":0.00035401358,"threshold_uncertainty_score":0.040908396},"labels":[],"label_agreement":null},{"id":"W1547770291","doi":"10.1086/317887","title":"The Peak Brightness and Spatial Distribution of Asymptotic Giant Branch Stars Near the Nucleus of M32","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Asymptotic giant branch; Stars; Brightness; Galaxy; Local Group; Surface brightness; Metallicity; Elliptical galaxy; Horizontal branch","score_opus":0.0038792336549411635,"score_gpt":0.18947201002950484,"score_spread":0.18559277637456367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1547770291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999496,0.000033435583,0.00004766552,0.0000054515453,2.6087952e-7,5.7092404e-7,0.000036989637,0.0000059193403,0.00037372872],"genre_scores_gemma":[0.99961543,0.000017630833,0.00011226207,0.000002243284,0.0000013572303,9.958301e-7,0.00010217017,0.0000030452527,0.00014488028],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995315,0.0000045887596,0.000002560116,0.000016601445,0.000007826189,0.00001534206],"domain_scores_gemma":[0.99969316,0.000039230836,0.00009238809,0.000027199087,0.000054901142,0.00009308952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106341315,0.00012002415,0.00016683577,0.0008224483,0.0002459018,0.0002646975,0.00014936965,0.0002235129,0.0011120865],"category_scores_gemma":[0.000519145,0.0001270835,0.000099213066,0.00035112113,0.00023488485,0.00025045525,0.00043383843,0.000109019515,0.0004541308],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046394914,0.0000335412,0.80764997,0.000043034375,0.000024405723,0.00043600306,0.0011199476,0.00043238563,0.17851847,0.00033920284,0.0002412409,0.010697801],"study_design_scores_gemma":[0.0000037079885,0.00004653302,0.99767596,0.000002898396,0.0000034546472,0.0003173702,0.0001438401,0.00023035594,0.0013450633,0.0000593607,0.00016877889,0.000002726751],"about_ca_topic_score_codex":0.0023084613,"about_ca_topic_score_gemma":0.0032675143,"teacher_disagreement_score":0.0023084613,"about_ca_system_score_codex":0.00020867665,"about_ca_system_score_gemma":0.00008964086,"threshold_uncertainty_score":0.004590094},"labels":[],"label_agreement":null},{"id":"W1548044706","doi":"10.1088/0004-637x/745/1/30","title":"THE MERGER HISTORY, ACTIVE GALACTIC NUCLEUS, AND DWARF GALAXIES OF HICKSON COMPACT GROUP 59","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Manitoba; Western University","funders":"","keywords":"Globular cluster; Galaxy group; Dwarf galaxy; Star formation; Galaxy; Active galactic nucleus; Compact group; Elliptical galaxy; Galaxy cluster","score_opus":0.014204214691005867,"score_gpt":0.20503641996236283,"score_spread":0.19083220527135697,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1548044706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991007,0.00009966738,0.000041167365,0.000013144512,0.000001286498,0.0000019695426,0.000046575835,0.00000236157,0.0006930421],"genre_scores_gemma":[0.9995828,0.00004227513,0.00005072188,0.000008264713,0.0000040918717,9.294618e-7,0.00011852125,0.0000017695169,0.00019068483],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990356,0.000008457545,0.0000063436946,0.000027624796,0.000026048689,0.000027922506],"domain_scores_gemma":[0.9995757,0.00003828073,0.00020854051,0.0000245485,0.000027775772,0.00012515385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018545178,0.00015105201,0.00014833592,0.0011031107,0.00039390137,0.00054142065,0.00019938436,0.00018904712,0.00091444637],"category_scores_gemma":[0.00067129475,0.00009699574,0.0001067008,0.00051661686,0.00048289046,0.0004561376,0.0005620782,0.00018439154,0.00022777429],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010618544,0.000032905537,0.9872196,0.000008579332,0.000017222314,0.00021539483,0.0005148755,0.0000615377,0.0071250997,0.00035609974,0.00010371892,0.004238841],"study_design_scores_gemma":[0.000002109705,0.0000277008,0.9990238,0.0000019872975,0.0000064732867,0.00021019315,0.00013419302,0.000064894106,0.0002354761,0.00007167343,0.00021954835,0.0000019118293],"about_ca_topic_score_codex":0.005717573,"about_ca_topic_score_gemma":0.007228875,"teacher_disagreement_score":0.005717573,"about_ca_system_score_codex":0.00027659268,"about_ca_system_score_gemma":0.00009689488,"threshold_uncertainty_score":0.011368573},"labels":[],"label_agreement":null},{"id":"W1550314177","doi":"10.1088/0004-637x/697/2/l162","title":"SELF-GRAVITY AND ANGULAR MOMENTUM TRANSPORT IN EXTENDED GALACTIC DISKS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Differential rotation; Angular momentum; Interstellar medium; Star formation; Turbulence; Specific relative angular momentum; Angular velocity; Gravitation; Cosmic ray; Rotation (mathematics)","score_opus":0.00629938865501578,"score_gpt":0.2336349670062168,"score_spread":0.22733557835120102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1550314177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991242,0.0000576579,0.0003916133,0.000011656789,0.0000016460912,0.0000011419563,0.000012173389,0.0000112233065,0.00038867156],"genre_scores_gemma":[0.99968946,0.000028759792,0.00016718924,0.000002701082,9.56987e-7,9.418728e-7,0.000014003991,0.000003785741,0.000092262366],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999671,0.0000050815493,0.000002683085,0.000007968521,0.0000062269232,0.000010884033],"domain_scores_gemma":[0.99983275,0.00005284271,0.000042911804,0.000022104825,0.000019557734,0.000029850382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000808186,0.00027005607,0.0002163969,0.00030076085,0.0002386937,0.0006840462,0.00031868578,0.00022054095,0.00064075226],"category_scores_gemma":[0.00061573996,0.00012405218,0.00018757641,0.00025545247,0.0004780304,0.0005251459,0.00057386135,0.00016472615,0.000059382877],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055694365,0.00018845015,0.13073598,0.00010503015,0.00016059601,0.0010246763,0.0007177344,0.7483931,0.09803121,0.009188625,0.00022854285,0.010669177],"study_design_scores_gemma":[0.00013114193,0.00021281018,0.057847876,0.000015023993,0.000045142293,0.00018695318,0.0002785626,0.920499,0.016170688,0.0038668115,0.0007071093,0.0000388162],"about_ca_topic_score_codex":0.004186838,"about_ca_topic_score_gemma":0.0022704634,"teacher_disagreement_score":0.004186838,"about_ca_system_score_codex":0.0003980831,"about_ca_system_score_gemma":0.00019107916,"threshold_uncertainty_score":0.008324921},"labels":[],"label_agreement":null},{"id":"W1550824617","doi":"10.1086/320668","title":"Detection of C<sub>3</sub>in Diffuse Interstellar Clouds","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":150,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Polyatomic ion; Interstellar medium; Interstellar cloud; Molecular cloud; Cosmochemistry; Carbon fibers; Atomic physics; Stars; Ion; Galaxy; Composite number","score_opus":0.008614807710100049,"score_gpt":0.2189097258885941,"score_spread":0.21029491817849405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1550824617","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978669,0.00018125381,0.00013428404,0.000031704047,0.0000020878704,0.0000036572574,0.00021035397,0.0000110687815,0.0015586346],"genre_scores_gemma":[0.9991273,0.00009012374,0.00021828646,0.000035344063,0.000005128614,0.000002964183,0.00028999784,0.000002799928,0.00022800406],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998784,0.0000049545047,0.000005089091,0.00003682621,0.000034304765,0.000040393337],"domain_scores_gemma":[0.99950576,0.00005044057,0.00014741422,0.000035209767,0.00010646471,0.00015471214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110826135,0.00016881622,0.00015975769,0.00085033104,0.00052020676,0.0005775639,0.0002532696,0.0002803705,0.0010096085],"category_scores_gemma":[0.000459605,0.00014581265,0.00009599104,0.00070086744,0.00046847365,0.00021738974,0.00042394942,0.0002746345,0.00021778766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040479007,0.000051462695,0.73967975,0.00005520757,0.000054025153,0.0003503694,0.00028841043,0.00018429851,0.24192591,0.0007228107,0.0003422397,0.015940756],"study_design_scores_gemma":[0.0000062308795,0.000042475935,0.98926187,0.0000082409115,0.000021114525,0.0003642728,0.00017391016,0.00022503267,0.008913733,0.00021465006,0.0007635318,0.000005042446],"about_ca_topic_score_codex":0.013574001,"about_ca_topic_score_gemma":0.028314302,"teacher_disagreement_score":0.013574001,"about_ca_system_score_codex":0.00044722826,"about_ca_system_score_gemma":0.00026016237,"threshold_uncertainty_score":0.026989996},"labels":[],"label_agreement":null},{"id":"W1552565640","doi":"10.1088/0004-637x/811/1/52","title":"THE DETECTION OF A SN IIn IN OPTICAL FOLLOW-UP OBSERVATIONS OF ICECUBE NEUTRINO EVENTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Planning and Budgeting Committee of the Council for Higher Education of Israel; Science Mission Directorate; Smithsonian Astrophysical Observatory; Office of Science; Office of Polar Programs; Max-Planck-Institut für Astronomie; Marsden Fund; Helmholtz Alliance for Astroparticle Physics; Eötvös Loránd Tudományegyetem; College of Engineering, Michigan State University; Knut och Alice Wallenbergs Stiftelse; Israel Science Foundation; Natural Sciences and Engineering Research Council of Canada; Bundesministerium für Bildung und Forschung; National Central University; Ohio State University; National Research Foundation of Korea; Fonds De La Recherche Scientifique - FNRS; Deutsche Forschungsgemeinschaft; Queen's University Belfast; National Research Foundation; Vlaamse regering; Weizmann Institute of Science; University of Oxford; University of Leicester; Durham University; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; York University; Space Telescope Science Institute; Western Canada Research Grid; Japan Society for the Promotion of Science; Queen's University; Harvard University; Polarforskningssekretariatet; Carnegie Mellon University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Vetenskapsrådet; Israeli Centers for Research Excellence; Yale University; University of Wisconsin-Madison; U.S. Department of Energy; Smithsonian Institution; California Institute of Technology; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; W. M. Keck Foundation; University of Portsmouth; New Mexico State University; Fonds Wetenschappelijk Onderzoek; Vanderbilt University; Compute Canada; Belgian Federal Science Policy Office; National Science Foundation","keywords":"Physics; Neutrino; Supernova; Astrophysics; Redshift; Luminosity; Ejecta; Galaxy; Observatory; Gamma-ray burst; Neutrino astronomy; Neutrino detector; Astronomy; Neutrino oscillation; Particle physics","score_opus":0.024320314446018662,"score_gpt":0.2414868903487322,"score_spread":0.21716657590271354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1552565640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.984639,0.00031680183,0.0008732922,0.00009301734,0.000079480495,0.00006198891,0.0040262328,0.00004742961,0.009862821],"genre_scores_gemma":[0.98666966,0.00024348467,0.0018101246,0.00015064438,0.00008456349,0.00006237147,0.008976252,0.000031288164,0.0019716497],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997125,0.000030151194,0.000022150065,0.00010417346,0.000083152125,0.00004782325],"domain_scores_gemma":[0.9991161,0.00009402328,0.00041677657,0.00007481676,0.00019875326,0.000099509736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006213522,0.00023090001,0.00016812755,0.0009867328,0.00043024772,0.00076920056,0.00022694726,0.00025585832,0.0011303977],"category_scores_gemma":[0.0014867228,0.00013397739,0.00019094549,0.0005879113,0.00024133884,0.00023017684,0.00078769255,0.00022936823,0.00032746128],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040042086,0.00004613308,0.9797346,0.0000472125,0.00006765562,0.0005678699,0.00029750905,0.00021001362,0.0047112545,0.0002634603,0.003040689,0.010613261],"study_design_scores_gemma":[0.000008735385,0.000037806727,0.99183196,0.000030412011,0.000042098087,0.0006321854,0.00020046369,0.0004664189,0.0014943848,0.00010847724,0.0051391115,0.00000799326],"about_ca_topic_score_codex":0.015018175,"about_ca_topic_score_gemma":0.03238397,"teacher_disagreement_score":0.015018175,"about_ca_system_score_codex":0.0006131136,"about_ca_system_score_gemma":0.00030166027,"threshold_uncertainty_score":0.02986151},"labels":[],"label_agreement":null},{"id":"W1555897420","doi":"10.1086/504888","title":"The Cosmic Reionization History as Revealed by the Cosmic Microwave Background Doppler–21 cm Correlation","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; Cosmic microwave background; Physics; Astrophysics; Anisotropy; Redshift; Doppler effect; Polarization (electrochemistry); Ionization; Cosmic variance; Universe; Cosmology; Astronomy; Galaxy; Optics; Ion; Chemistry; Quantum mechanics","score_opus":0.006734499884279924,"score_gpt":0.21718291957890107,"score_spread":0.21044841969462114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1555897420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98795086,0.0003032444,0.0052928133,0.00009288835,0.0000089825635,0.0000036759188,0.00040225993,0.00011222954,0.0058331024],"genre_scores_gemma":[0.9988881,0.00007492363,0.0006362477,0.000009879846,0.000010924047,0.000001999652,0.00017102544,0.000010166457,0.00019678434],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984145,0.000024774725,0.0000051836637,0.000055533226,0.000034430726,0.000038645663],"domain_scores_gemma":[0.9989519,0.0002135581,0.00052829727,0.0001331545,0.0000844135,0.00008863871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027746402,0.00022329562,0.00014688732,0.0008070897,0.00016438644,0.0006588921,0.00018548484,0.00017778276,0.0011510641],"category_scores_gemma":[0.0019728641,0.00010132125,0.00013271009,0.0012121772,0.00033682786,0.0004765604,0.00060447166,0.0002973957,0.00019746911],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021909086,0.000031140975,0.84704393,0.00007764553,0.00017805916,0.0006473334,0.00043394227,0.02432772,0.03548162,0.033296283,0.0015319466,0.05673125],"study_design_scores_gemma":[0.0000030907736,0.000024272083,0.9731259,0.00000825542,0.000021937243,0.00023707571,0.00005795618,0.017943496,0.0025090133,0.0038746584,0.0021728491,0.000021399192],"about_ca_topic_score_codex":0.0018847183,"about_ca_topic_score_gemma":0.0011261195,"teacher_disagreement_score":0.0018847183,"about_ca_system_score_codex":0.00031406854,"about_ca_system_score_gemma":0.00012324665,"threshold_uncertainty_score":0.0038506389},"labels":[],"label_agreement":null},{"id":"W1563243244","doi":"10.1088/0004-637x/728/1/38","title":"AEGIS: DEMOGRAPHICS OF X-RAY AND OPTICALLY SELECTED ACTIVE GALACTIC NUCLEI","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Active galactic nucleus; Galaxy; Redshift; Astronomy; Emission spectrum; Star formation; Luminous infrared galaxy; Demographics; Population; Doubly ionized oxygen; Line (geometry); Spectral line; Medicine","score_opus":0.009110601166089926,"score_gpt":0.19933507921962926,"score_spread":0.19022447805353934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1563243244","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88795954,0.00045499104,0.0029112473,0.00014076791,0.00003415819,0.0002171967,0.091881216,0.00028308888,0.01611781],"genre_scores_gemma":[0.85899353,0.0007364382,0.009923241,0.00017197464,0.00005402301,0.00041752035,0.12251232,0.00010103362,0.007089833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998085,0.00002516942,0.000028421744,0.00006337942,0.00004823906,0.000026402491],"domain_scores_gemma":[0.99935514,0.000050017738,0.00028349087,0.0000620832,0.00012213156,0.00012711741],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033316,0.0002563462,0.0001982806,0.0027358881,0.0002070663,0.0005317661,0.00029795506,0.000109874476,0.0038273805],"category_scores_gemma":[0.00079432037,0.00012442631,0.00013811546,0.0013377896,0.00012873935,0.000499863,0.00064852595,0.00018550534,0.001634713],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000077863355,0.000019642455,0.967486,0.00004238334,0.000037904276,0.000091840615,0.0003101537,0.00029904972,0.004162653,0.0009935875,0.0051424797,0.021336483],"study_design_scores_gemma":[0.0000044372587,0.000019241663,0.98641276,0.0000081711105,0.0000072584903,0.00021726661,0.00017872188,0.00041510654,0.00042999635,0.00014281219,0.012159539,0.0000046069094],"about_ca_topic_score_codex":0.016113536,"about_ca_topic_score_gemma":0.022466443,"teacher_disagreement_score":0.016113536,"about_ca_system_score_codex":0.00045054013,"about_ca_system_score_gemma":0.00029767194,"threshold_uncertainty_score":0.032039523},"labels":[],"label_agreement":null},{"id":"W1569438225","doi":"10.1088/0004-637x/801/1/63","title":"ALMA MULTI-LINE IMAGING OF THE NEARBY STARBURST NGC 253","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Isotopologue; Galaxy; Line (geometry); Hydrogen molecule; Luminosity; H II region; Hydrogen; Molecular cloud","score_opus":0.023971521756831163,"score_gpt":0.26676716906774806,"score_spread":0.2427956473109169,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1569438225","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944877,0.00021358956,0.0015321679,0.000057917783,0.000007513542,0.0000076273523,0.00057489186,0.00014140976,0.0029772678],"genre_scores_gemma":[0.9948171,0.00008374554,0.0039157798,0.000048261703,0.000015124676,0.000009739907,0.00032634565,0.000012366176,0.0007714287],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995446,0.0000031904772,0.0000022152458,0.000019991001,0.00000982396,0.000010303309],"domain_scores_gemma":[0.9999031,0.000014730786,0.000020151214,0.000015261588,0.000013939447,0.000032860786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000089176036,0.000108519176,0.00011041349,0.0004519344,0.00021755252,0.00020775133,0.00025337853,0.00024331288,0.0020528291],"category_scores_gemma":[0.00010849496,0.000104333645,0.00012885209,0.00018341362,0.00008328745,0.0001472056,0.0001645136,0.00015619429,0.00031290922],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002700882,0.00011130296,0.08056349,0.00006249559,0.000052381558,0.0008341042,0.00019954065,0.0016132718,0.89455014,0.0003265902,0.0012548241,0.02016183],"study_design_scores_gemma":[0.000025267589,0.00022642475,0.95658386,0.000017579934,0.000047603906,0.0013190686,0.00020591058,0.007487682,0.030560732,0.00019845593,0.0033114546,0.0000160689],"about_ca_topic_score_codex":0.003777446,"about_ca_topic_score_gemma":0.009987025,"teacher_disagreement_score":0.003777446,"about_ca_system_score_codex":0.00024137611,"about_ca_system_score_gemma":0.00008016044,"threshold_uncertainty_score":0.0075109005},"labels":[],"label_agreement":null},{"id":"W1569717828","doi":"10.1088/0004-637x/726/2/67","title":"MASS TRANSFER IN BINARY STARS USING SMOOTHED PARTICLE HYDRODYNAMICS. II. ECCENTRIC BINARIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Binary number; Eccentricity (behavior); Stars; Smoothed-particle hydrodynamics; Binary star; Roche lobe; Common envelope; Mass transfer; Population; Orbital eccentricity","score_opus":0.009735681623247254,"score_gpt":0.23182956023999432,"score_spread":0.22209387861674706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1569717828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9611575,0.00021962055,0.035298694,0.00014548781,0.000025679292,0.00004937969,0.0002181616,0.00024278408,0.0026427202],"genre_scores_gemma":[0.9933622,0.00007274165,0.005720873,0.00003587389,0.000014419855,0.000027302114,0.00013184328,0.00004630757,0.0005884406],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999206,0.000021388722,0.000005652172,0.0000120834175,0.000019115218,0.000021267293],"domain_scores_gemma":[0.99948275,0.00017875434,0.00013854992,0.00005334433,0.000055481287,0.000091078415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037331737,0.0004007778,0.00048782272,0.0005446359,0.00045644795,0.00066566776,0.0006939053,0.0006286836,0.00081513956],"category_scores_gemma":[0.001444839,0.000305422,0.0005242412,0.0004879876,0.00084391795,0.00070496474,0.00069819513,0.0004403514,0.00013803845],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009773615,0.00007501621,0.010671164,0.00003142711,0.000061541614,0.00010290107,0.00012467439,0.97606975,0.0038357761,0.0060638664,0.0002153367,0.002650669],"study_design_scores_gemma":[0.00002093861,0.000013203677,0.001588658,0.0000016693979,0.000003939471,0.00001129564,0.00001253616,0.99654573,0.00028412204,0.0013828666,0.00012899037,0.0000061102014],"about_ca_topic_score_codex":0.014580427,"about_ca_topic_score_gemma":0.006488497,"teacher_disagreement_score":0.014580427,"about_ca_system_score_codex":0.0011493608,"about_ca_system_score_gemma":0.00069382496,"threshold_uncertainty_score":0.028991103},"labels":[],"label_agreement":null},{"id":"W1572376656","doi":"10.1086/524677","title":"An Improved Photometric Calibration of the Sloan Digital Sky Survey Imaging Data","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomical Observations and Instrumentation","field":"Engineering","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Los Alamos National Laboratory; U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; University of Cambridge; New Mexico State University; University of Portsmouth; Universität Basel; University of Pittsburgh; Johns Hopkins University; Ohio State University; U.S. Department of Energy; Princeton University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Drexel University; National Aeronautics and Space Administration; Case Western Reserve University","keywords":"Sky; Calibration; Remote sensing; Observatory; Point (geometry); Computer science; Environmental science; Physics; Optics; Astrophysics; Geology; Mathematics","score_opus":0.025671939524525834,"score_gpt":0.22875024425122514,"score_spread":0.2030783047266993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1572376656","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01604246,0.00019292202,0.971584,0.00019250777,0.00012308142,0.00008105725,0.0011898595,0.007055412,0.0035386044],"genre_scores_gemma":[0.061497696,0.00013733488,0.93053323,0.000120342775,0.000068457775,0.00011709527,0.0035006583,0.0009107705,0.0031143816],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99741614,0.00040048893,0.00013475488,0.0007084038,0.00116797,0.00017225652],"domain_scores_gemma":[0.99775285,0.00012829273,0.00020549352,0.0006591338,0.0011861359,0.00006816981],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002604923,0.0007522624,0.00056686543,0.0029677108,0.0009130869,0.001599213,0.001201295,0.0006136488,0.0028703287],"category_scores_gemma":[0.0074831415,0.0007138613,0.00074053847,0.0034618918,0.00036330026,0.0014033768,0.0021118743,0.0017205537,0.0045798863],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010753384,0.00014326056,0.025489733,0.000096964905,0.0001179296,0.00006932049,0.00040231927,0.05502719,0.035980355,0.020302119,0.04135427,0.8209091],"study_design_scores_gemma":[0.000087014436,0.00008427184,0.05022288,0.000078617886,0.00008114676,0.00040717536,0.00020136141,0.71698153,0.052352156,0.022976743,0.15632358,0.00020363826],"about_ca_topic_score_codex":0.0124205155,"about_ca_topic_score_gemma":0.014361302,"teacher_disagreement_score":0.0124205155,"about_ca_system_score_codex":0.0010386315,"about_ca_system_score_gemma":0.0015285711,"threshold_uncertainty_score":0.02469641},"labels":[],"label_agreement":null},{"id":"W1575104529","doi":"10.1088/0004-637x/763/1/63","title":"RADIO ACTIVE GALAXY NUCLEI IN GALAXY CLUSTERS: HEATING HOT ATMOSPHERES AND DRIVING SUPERMASSIVE BLACK HOLE GROWTH OVER COSMIC TIME","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Supermassive black hole; Luminosity; Redshift; Galaxy cluster; Radio galaxy; Astronomy; Galaxy; Cluster (spacecraft); Intracluster medium; Black hole (networking)","score_opus":0.004606103865960342,"score_gpt":0.19527509707764706,"score_spread":0.19066899321168673,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1575104529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99913603,0.00013590643,0.00021812187,0.000015635269,0.0000014256638,0.0000025076743,0.00013511127,0.000007537749,0.00034771863],"genre_scores_gemma":[0.99948394,0.00006544293,0.00015531843,0.0000042209613,0.0000057642114,0.0000017110103,0.00015741431,0.0000028558984,0.00012329589],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991643,0.000010520923,0.000004011071,0.0000290456,0.000015636206,0.000024329778],"domain_scores_gemma":[0.9991223,0.00017766033,0.00043623426,0.000069660695,0.000053135944,0.00014092379],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002666268,0.0003056052,0.00016589003,0.0009034571,0.00018730744,0.0005781245,0.0003753697,0.00025532732,0.0012783611],"category_scores_gemma":[0.0011413111,0.00017267543,0.00034232784,0.00050881034,0.0003507312,0.0004660446,0.00043928795,0.00018773263,0.00021760169],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000585459,0.000013226788,0.989883,0.000018883653,0.000046455574,0.000109963956,0.00025051617,0.0036987842,0.0028494967,0.00040473122,0.00007634143,0.0025900882],"study_design_scores_gemma":[0.0000015760114,0.000013416233,0.9961343,0.0000017459453,0.000011061772,0.000054262786,0.00005774646,0.0031349414,0.00030296136,0.0001661398,0.000119255754,0.0000026919715],"about_ca_topic_score_codex":0.011450814,"about_ca_topic_score_gemma":0.010807783,"teacher_disagreement_score":0.011450814,"about_ca_system_score_codex":0.0005351849,"about_ca_system_score_gemma":0.00011399231,"threshold_uncertainty_score":0.022768378},"labels":[],"label_agreement":null},{"id":"W1575190847","doi":"10.1088/0004-637x/807/1/85","title":"SEEDING THE PREGENETIC EARTH: METEORITIC ABUNDANCES OF NUCLEOBASES AND POTENTIAL REACTION PATHWAYS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Origins and Evolution of Life","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of British Columbia","funders":"","keywords":"Nucleobase; Murchison meteorite; Meteorite; Uracil; Chondrite; Chemistry; Thymine; Astrobiology; DNA; Biology; Biochemistry","score_opus":0.020672537802828125,"score_gpt":0.23362885381372592,"score_spread":0.2129563160108978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1575190847","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7878141,0.17128514,0.01141803,0.00039946652,0.00019540651,0.000069876434,0.0043481877,0.00032259917,0.024147201],"genre_scores_gemma":[0.9190286,0.06157973,0.008050168,0.00008595419,0.00007445997,0.000025449963,0.0045431214,0.00007757846,0.006534883],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99988353,0.000011287534,0.00000824031,0.000048067664,0.000034353427,0.000014584576],"domain_scores_gemma":[0.99980086,0.000036439156,0.00006583872,0.000012188559,0.000062850406,0.000021903343],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023795609,0.0003696261,0.00027819432,0.0010889993,0.0002847334,0.00091639097,0.00027888024,0.00030878786,0.001523684],"category_scores_gemma":[0.00043256138,0.0001440898,0.00018193676,0.0013408841,0.0002565425,0.00087703904,0.00032176214,0.00023010577,0.00055368536],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089957844,0.000116557014,0.28786382,0.0076394808,0.00039227068,0.0023972325,0.001280256,0.006153715,0.38614586,0.015583925,0.0036327282,0.28789455],"study_design_scores_gemma":[0.000025100018,0.00068012404,0.50547886,0.0006543393,0.00035003427,0.003694603,0.0017607214,0.0050673126,0.16662748,0.0136002535,0.30198216,0.00007892624],"about_ca_topic_score_codex":0.0019207854,"about_ca_topic_score_gemma":0.0035909044,"teacher_disagreement_score":0.0019207854,"about_ca_system_score_codex":0.0004602756,"about_ca_system_score_gemma":0.00030974406,"threshold_uncertainty_score":0.0050972104},"labels":[],"label_agreement":null},{"id":"W1576269525","doi":"10.1086/309298","title":"The Propagation of Magnetocentrifugally Launched Jets. I.","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Jet (fluid); Magnetohydrodynamics; RADIUS; Mechanics; Magnetic field; Core (optical fiber); Stratification (seeds); Computational physics; Launched; Turbulence; Classical mechanics; Optics","score_opus":0.0037153767114087737,"score_gpt":0.1995424974222876,"score_spread":0.19582712071087882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1576269525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9667276,0.00033098293,0.012734313,0.0005408293,0.00009193286,0.00006157107,0.00069997954,0.00027909604,0.018533653],"genre_scores_gemma":[0.99436486,0.00012783466,0.0032577482,0.00007152993,0.000013392671,0.000022724524,0.0003852801,0.00004438854,0.0017122979],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99990344,0.000022348762,0.0000040328896,0.00001366619,0.000018989718,0.000037509355],"domain_scores_gemma":[0.9994259,0.00026789005,0.00009635896,0.00003129323,0.00007524545,0.0001032754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026191998,0.00036221332,0.00028882723,0.0003363241,0.0005179368,0.0009599366,0.0006633897,0.0009156945,0.0020951878],"category_scores_gemma":[0.0020107392,0.00023854147,0.00035725697,0.00038284625,0.0005973433,0.0006853124,0.0006876375,0.0006974742,0.0002208427],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021091675,0.00011336416,0.008491284,0.000031632007,0.000046479767,0.00035807118,0.00019344235,0.9775997,0.0023516868,0.0065240585,0.0010206238,0.0030587038],"study_design_scores_gemma":[0.000078052464,0.000057478068,0.0017288654,0.000008932069,0.0000104011015,0.000032101692,0.00006899092,0.99544585,0.0007384146,0.0010744355,0.0007450139,0.000011490001],"about_ca_topic_score_codex":0.027599992,"about_ca_topic_score_gemma":0.0119545115,"teacher_disagreement_score":0.027599992,"about_ca_system_score_codex":0.000961113,"about_ca_system_score_gemma":0.00069881853,"threshold_uncertainty_score":0.054878652},"labels":[],"label_agreement":null},{"id":"W1578263179","doi":"10.1086/318919","title":"Submillimeter Imaging of a Protocluster Region at [CLC][ITAL]z[/ITAL][/CLC] = 3.09","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"James Clerk Maxwell Telescope; Bolometer; Telescope; Flux (metallurgy); Serpens; Optical depth; Detector; Field (mathematics)","score_opus":0.009113344860982468,"score_gpt":0.21409546640303648,"score_spread":0.204982121542054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1578263179","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9858431,0.00013824542,0.0009097046,0.00014120147,0.000022086002,0.000022417082,0.0018207623,0.00021996468,0.010882491],"genre_scores_gemma":[0.9899479,0.0000918261,0.0046415883,0.00013532155,0.000022746377,0.00001751596,0.002917028,0.00004706327,0.0021789134],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999454,0.0000017710419,0.0000014708338,0.000012134448,0.000019524343,0.000019660592],"domain_scores_gemma":[0.9997993,0.000011564093,0.00004403538,0.000022865373,0.0000582118,0.00006412239],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011791953,0.00010326073,0.000120909805,0.00051544054,0.00043597515,0.00036971827,0.00047533002,0.00024851237,0.0019329893],"category_scores_gemma":[0.00017262305,0.00014269096,0.00012434328,0.0003876895,0.000119239085,0.00014649832,0.00036399497,0.0003452489,0.0006342445],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038978286,0.00017561165,0.17790607,0.00006873721,0.000077851284,0.0016218593,0.00048519022,0.001024176,0.7787165,0.0013540634,0.008867788,0.02931237],"study_design_scores_gemma":[0.000016607688,0.0000474598,0.98071253,0.000009679236,0.000015847907,0.0004818673,0.00007763387,0.0015386225,0.012311663,0.00012743426,0.0046523637,0.000008362977],"about_ca_topic_score_codex":0.013085777,"about_ca_topic_score_gemma":0.026253084,"teacher_disagreement_score":0.013085777,"about_ca_system_score_codex":0.00043818026,"about_ca_system_score_gemma":0.0002491819,"threshold_uncertainty_score":0.026019216},"labels":[],"label_agreement":null},{"id":"W1578419887","doi":"10.1088/0004-637x/804/2/150","title":"CHANGING PHASES OF ALIEN WORLDS: PROBING ATMOSPHERES OF<i>KEPLER</i>PLANETS WITH HIGH-PRECISION PHOTOMETRY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":199,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Light curve; Photometry (optics); Brightness; Amplitude; Planetary system; Geometric albedo; Exoplanet; Asteroid","score_opus":0.014902129647418796,"score_gpt":0.23524316838466838,"score_spread":0.22034103873724958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1578419887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981896,0.00006885094,0.000648964,0.000014608911,0.0000010146254,0.000003308692,0.00036385568,0.000038121783,0.00067152723],"genre_scores_gemma":[0.99835867,0.00003585422,0.0010353468,0.0000063321663,0.0000029258074,0.0000030560664,0.00049022195,0.000010758134,0.000056809935],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988294,0.00001634298,0.0000053957606,0.00004288843,0.000025552765,0.000026908141],"domain_scores_gemma":[0.9994729,0.00013350592,0.0001822055,0.00007544121,0.00003859629,0.0000974334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020297804,0.00019225646,0.00020930675,0.00088890066,0.00040077345,0.0006555067,0.00024030078,0.00026403536,0.00057922734],"category_scores_gemma":[0.00083730416,0.00021762408,0.0002207787,0.0009091929,0.0002744994,0.0005803467,0.0007343849,0.0003051214,0.00016319091],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020480737,0.00006484499,0.9382867,0.000050965027,0.00012761803,0.000110583955,0.0007787817,0.0027080646,0.03783346,0.00035069048,0.00039439587,0.019089073],"study_design_scores_gemma":[0.000005994342,0.000043519754,0.99074566,0.0000039172373,0.000023371238,0.00013153264,0.00018385549,0.0048564337,0.002693417,0.00021354252,0.0010891665,0.000009442618],"about_ca_topic_score_codex":0.0025555901,"about_ca_topic_score_gemma":0.004719948,"teacher_disagreement_score":0.0025555901,"about_ca_system_score_codex":0.0002488716,"about_ca_system_score_gemma":0.00011426808,"threshold_uncertainty_score":0.005081475},"labels":[],"label_agreement":null},{"id":"W1581696452","doi":"10.1088/0004-637x/781/2/101","title":"<i>HERSCHEL</i>-SPIRE FOURIER TRANSFORM SPECTROMETER OBSERVATIONS OF EXCITED CO AND [C I] IN THE ANTENNAE (NGC 4038/39): WARM AND COLD MOLECULAR GAS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Max-Planck-Institut für Astronomie; Centre National de la Recherche Scientifique; Università degli Studi di Padova; KU Leuven; Imperial College London; Agenzia Spaziale Italiana; Jet Propulsion Laboratory; Bundesministerium für Verkehr, Innovation und Technologie; Centre National d’Etudes Spatiales; National Aeronautics and Space Administration; Fonds Wetenschappelijk Onderzoek; Cardiff University; California Institute of Technology; University of Lethbridge; Vlaamse regering; University of Sussex","keywords":"Radiative transfer; Excited state; Flux (metallurgy); Abundance (ecology); Atmospheric radiative transfer codes; Fourier transform; Radiative cooling; Spectroscopy","score_opus":0.008962392221617372,"score_gpt":0.2071987594731675,"score_spread":0.1982363672515501,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1581696452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97609216,0.0002019628,0.00040427723,0.00031606868,0.000015646794,0.000025178519,0.011683267,0.00040148286,0.010860019],"genre_scores_gemma":[0.98546046,0.0001711816,0.0026587946,0.00015934803,0.00004773079,0.000024094876,0.008973335,0.00006846843,0.0024365324],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998604,0.0000087570015,0.000004913371,0.000040347604,0.000045216442,0.000040441675],"domain_scores_gemma":[0.9998091,0.000013382883,0.00006489032,0.00002866148,0.000020088248,0.000063887885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016380157,0.00035703107,0.00022583196,0.0015627912,0.00053947576,0.0003349389,0.00047128665,0.0004551228,0.0036206723],"category_scores_gemma":[0.00021240054,0.0001745936,0.00030184322,0.0009967402,0.00027127846,0.00029137146,0.00056997605,0.00027200623,0.0007874434],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051308447,0.00028011255,0.66403013,0.00016510872,0.0003199099,0.0026522586,0.0009434867,0.008510628,0.25503385,0.0016818137,0.028335014,0.037534446],"study_design_scores_gemma":[0.000040122843,0.000048383863,0.98459977,0.000013877831,0.000026688886,0.00049492536,0.00011455481,0.0018227006,0.0059419964,0.00026972123,0.0065979445,0.00002934165],"about_ca_topic_score_codex":0.02722053,"about_ca_topic_score_gemma":0.069374055,"teacher_disagreement_score":0.02722053,"about_ca_system_score_codex":0.0007951898,"about_ca_system_score_gemma":0.00027734155,"threshold_uncertainty_score":0.054124177},"labels":[],"label_agreement":null},{"id":"W1582823309","doi":"10.1086/309066","title":"Gas and Dust in NGC 7469: Submillimeter Imaging and CO<i>J</i> = 3–2","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; James Clerk Maxwell Telescope; Submillimeter Array; Astrophysics; Galaxy; Interstellar medium; Milky Way; Cosmic dust; Spiral galaxy; Luminous infrared galaxy; Bolometer; Infrared; Astronomy; Telescope; Star formation; Optics","score_opus":0.004834216974599421,"score_gpt":0.20144143527612537,"score_spread":0.19660721830152594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1582823309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978532,0.00012366952,0.000085539934,0.000033849432,0.000005317324,0.000003853839,0.00023778006,0.00003197309,0.0016248078],"genre_scores_gemma":[0.9990522,0.000055768553,0.0002933511,0.000026319392,0.000013849837,0.0000032078906,0.00034085853,0.0000050483955,0.00020935627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987376,0.0000046956784,0.0000031488214,0.000024446235,0.000023715944,0.00007032172],"domain_scores_gemma":[0.99984956,0.000009113664,0.000060926293,0.000009097096,0.000013563867,0.000057669942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006319863,0.00023442354,0.00021214836,0.0014223108,0.0006423821,0.00037211674,0.00030524007,0.00033247872,0.0014493495],"category_scores_gemma":[0.00010644978,0.00012888946,0.00014960313,0.0009005312,0.00023675238,0.000181745,0.00033647244,0.00020256064,0.00033937086],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046936973,0.00026929716,0.77057505,0.00006285232,0.00010204117,0.0036202192,0.00086198014,0.0015896868,0.19454482,0.0006504427,0.0032122373,0.024041904],"study_design_scores_gemma":[0.000004099674,0.00001991281,0.9974712,0.00000320381,0.0000084051935,0.0003255436,0.00009215339,0.00026971198,0.0008759018,0.000035959503,0.00088884035,0.0000051093434],"about_ca_topic_score_codex":0.04097451,"about_ca_topic_score_gemma":0.103759356,"teacher_disagreement_score":0.04097451,"about_ca_system_score_codex":0.00053289277,"about_ca_system_score_gemma":0.00020564454,"threshold_uncertainty_score":0.08147198},"labels":[],"label_agreement":null},{"id":"W1582934143","doi":"10.1088/0004-637x/809/1/40","title":"CLASSIFYING X-RAY BINARIES: A PROBABILISTIC APPROACH","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"","keywords":"Binary number; Boundary (topology); Neutron star; Compact star; Black hole (networking); Coordinate system; Probabilistic logic; Energy (signal processing); Bayesian probability; Galaxy","score_opus":0.043231387670454355,"score_gpt":0.2505874091614237,"score_spread":0.20735602149096932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1582934143","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.083618134,0.00060265703,0.90992224,0.0013131482,0.00005282779,0.00021441889,0.0005897488,0.0005056065,0.0031811765],"genre_scores_gemma":[0.7638066,0.00077149447,0.2294244,0.00035555512,0.0003764057,0.00034237566,0.0016105875,0.000100139405,0.0032124638],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9975694,0.0008622615,0.00016108266,0.00057401264,0.00063544686,0.000197733],"domain_scores_gemma":[0.9923233,0.0052712234,0.0008953661,0.0005606382,0.0006603382,0.00028919216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003905547,0.00071664643,0.0010798984,0.0057967855,0.0017729722,0.004183398,0.0037841506,0.0022914936,0.0026297548],"category_scores_gemma":[0.013511884,0.0009933118,0.0015822282,0.0027283812,0.0020069927,0.0036981744,0.0024990574,0.0020065268,0.00069886714],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035942005,0.0005608645,0.102890335,0.00025607125,0.00042898997,0.00057157903,0.001082229,0.5715685,0.0026466092,0.1452803,0.004097683,0.17025742],"study_design_scores_gemma":[0.000017866545,0.000025806703,0.004240531,0.000027311069,0.000032098098,0.00015312037,0.000098717035,0.93391263,0.00021841782,0.06037609,0.00086167594,0.000035676476],"about_ca_topic_score_codex":0.01254414,"about_ca_topic_score_gemma":0.012492017,"teacher_disagreement_score":0.01254414,"about_ca_system_score_codex":0.001518631,"about_ca_system_score_gemma":0.0015042137,"threshold_uncertainty_score":0.024942279},"labels":[],"label_agreement":null},{"id":"W1584216552","doi":"10.1088/0004-637x/694/2/1115","title":"AN ACCURATE DETERMINATION OF THE OPTICAL PERIODIC MODULATION IN THE X-RAY BINARY SAX J1808.4–3658","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Modulation (music); Binary number; Flux (metallurgy); Light curve; Binary star; Phase (matter); Consistency (knowledge bases); Millisecond pulsar","score_opus":0.014913561060163399,"score_gpt":0.25950603374428877,"score_spread":0.24459247268412537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1584216552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9837246,0.0010285426,0.007062052,0.00028304596,0.000117737516,0.00003003734,0.0005770173,0.00032247667,0.006854633],"genre_scores_gemma":[0.9939201,0.00014410868,0.0047735395,0.000044714536,0.000037321865,0.000012783494,0.0003943469,0.000035434165,0.00063755264],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999026,0.000012987016,0.0000055823125,0.000037451915,0.00002686431,0.0000145345075],"domain_scores_gemma":[0.99977154,0.00003707531,0.00005783728,0.00005292869,0.000039400016,0.000041252053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026226832,0.00020821158,0.00022551867,0.00086679665,0.00027910795,0.00065261434,0.00037153348,0.00045415873,0.0016290668],"category_scores_gemma":[0.0007012051,0.00033756628,0.00013318396,0.00041207037,0.00024992926,0.0004793861,0.0006419172,0.00046819614,0.0005644533],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012265227,0.00016764259,0.12314503,0.000386547,0.00008962604,0.00042240263,0.00055883423,0.0046881423,0.7373487,0.0061505483,0.0035454247,0.12227062],"study_design_scores_gemma":[0.00028405778,0.00032282624,0.8511015,0.00009547039,0.00015783127,0.0005876818,0.0002515329,0.058749117,0.07474173,0.0037898475,0.009851504,0.00006690712],"about_ca_topic_score_codex":0.0011102045,"about_ca_topic_score_gemma":0.0021488043,"teacher_disagreement_score":0.0016290668,"about_ca_system_score_codex":0.000295798,"about_ca_system_score_gemma":0.00021864612,"threshold_uncertainty_score":0.0054497123},"labels":[],"label_agreement":null},{"id":"W1585153339","doi":"10.1086/509315","title":"<i>MOST</i>Detects<i>g</i>‐Modes in the Late‐Type Be Star β Canis Minoris (B8 Ve)","year":2006,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; University of Toronto; Université du Québec à Montréal; Université de Montréal; Saint Mary's University; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Stars; Excited state; Amplitude; Star (game theory); Opacity; Astronomy; Optics; Atomic physics","score_opus":0.011388472655680862,"score_gpt":0.21647851307306873,"score_spread":0.20509004041738788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1585153339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99536824,0.00016578626,0.00054341654,0.000039737773,0.0000069627686,0.0000057868338,0.00011031893,0.00005180297,0.0037079828],"genre_scores_gemma":[0.9983828,0.00005165009,0.00081740785,0.000031961208,0.000008009382,0.0000031422976,0.00024149446,0.000009503941,0.0004540332],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992526,0.0000046272366,0.0000035121982,0.000025829731,0.000018789182,0.000022018039],"domain_scores_gemma":[0.99970514,0.00002881177,0.00009837667,0.000034183908,0.000059219772,0.00007429502],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012871738,0.0001904353,0.00012946542,0.0005780529,0.00029147812,0.0003438842,0.00027344673,0.00034995598,0.0015605206],"category_scores_gemma":[0.00033576667,0.0001526792,0.00008925736,0.00019807123,0.0002456108,0.00022683045,0.00029392436,0.00026258084,0.00033481664],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024250119,0.000056559456,0.41560268,0.000063156294,0.000034071563,0.00036149632,0.0002881825,0.00005915504,0.56406325,0.00029317595,0.0005457412,0.018390002],"study_design_scores_gemma":[0.000007567278,0.00021187072,0.94634634,0.000013870837,0.00003642683,0.0019887532,0.00012718252,0.0002844094,0.04802623,0.00014783825,0.0028003207,0.00000927586],"about_ca_topic_score_codex":0.0010796998,"about_ca_topic_score_gemma":0.0025640153,"teacher_disagreement_score":0.0015605206,"about_ca_system_score_codex":0.000101863756,"about_ca_system_score_gemma":0.000052513627,"threshold_uncertainty_score":0.005220413},"labels":[],"label_agreement":null},{"id":"W1589229034","doi":"10.1088/0004-637x/815/1/51","title":"INTERPRETING THE UNRESOLVED INTENSITY OF COSMOLOGICALLY REDSHIFTED LINE RADIATION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; Canadian Institute for Advanced Research","funders":"","keywords":"Intensity mapping; Background radiation; Radiant intensity; Spectral line; Radiation; Intensity (physics); Line (geometry); Spectral shape analysis","score_opus":0.01595191223559377,"score_gpt":0.23310036920158098,"score_spread":0.2171484569659872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1589229034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81467247,0.00045985178,0.17882936,0.00031848732,0.000035376328,0.000045564546,0.00073772774,0.00036944664,0.0045317495],"genre_scores_gemma":[0.96449804,0.00014715086,0.034026556,0.00009310403,0.000037232854,0.000024611316,0.00049689,0.00011796894,0.00055832113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991573,0.0002728142,0.0000345447,0.0002899974,0.00017581467,0.00006955114],"domain_scores_gemma":[0.9960632,0.0013239166,0.0009548367,0.0010314,0.00047733483,0.00014941244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026693437,0.00037129378,0.00036992345,0.0014819192,0.00037928327,0.0016654553,0.00072932884,0.0006688378,0.00097216084],"category_scores_gemma":[0.0091252485,0.00036916672,0.00035515835,0.0011968958,0.0010383021,0.0011880005,0.0010530319,0.0006640738,0.0002863991],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004851005,0.00020458612,0.6363657,0.00030999893,0.00040309085,0.00021284286,0.0019249592,0.033363387,0.18525536,0.034237552,0.0016124297,0.105624996],"study_design_scores_gemma":[0.0000319126,0.00011442814,0.82741857,0.000033780438,0.00016261393,0.00024662772,0.00055832876,0.102794364,0.03420067,0.02926012,0.0050959075,0.00008268315],"about_ca_topic_score_codex":0.003111041,"about_ca_topic_score_gemma":0.0024346055,"teacher_disagreement_score":0.003111041,"about_ca_system_score_codex":0.0006283347,"about_ca_system_score_gemma":0.00024778035,"threshold_uncertainty_score":0.014117062},"labels":[],"label_agreement":null},{"id":"W1589747147","doi":"10.1088/0004-637x/794/1/13","title":"SCALING OF OBSERVABLE PROPERTIES IN ROTATING STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Compute Canada","keywords":"Luminosity; Scaling; Observable; Stars; Spectral energy distribution; Plane (geometry); Distribution (mathematics); Distribution function; Range (aeronautics)","score_opus":0.020086940828575057,"score_gpt":0.2167861105904116,"score_spread":0.19669916976183655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1589747147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99472874,0.00009580279,0.0026641039,0.00002259908,0.000002522556,0.0000044383883,0.0001859401,0.00012515052,0.0021706945],"genre_scores_gemma":[0.99915886,0.000026444839,0.00052531116,0.0000024356075,0.000002697772,0.0000022168315,0.00020128448,0.000021661222,0.00005906116],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999808,0.000038886446,0.000013612857,0.000069850845,0.0000404509,0.000029235725],"domain_scores_gemma":[0.9983022,0.00060210656,0.0003557292,0.00036443816,0.00023298708,0.000142472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035107878,0.0003093651,0.00024904747,0.00095971406,0.00025485086,0.00088893366,0.00029451738,0.00026419025,0.0010117096],"category_scores_gemma":[0.0040688296,0.00018481047,0.00037585094,0.0006619195,0.0004516547,0.0005922119,0.00042015588,0.0002921985,0.0002837808],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041103238,0.00013690988,0.770526,0.000088411514,0.00015047181,0.0004989958,0.00050200726,0.12441184,0.06397586,0.008336673,0.0004822198,0.030479599],"study_design_scores_gemma":[0.0000191512,0.0001136645,0.7850609,0.000014307219,0.000034478446,0.00032187594,0.00016500846,0.2007702,0.008262769,0.0043410156,0.0008602087,0.000036370817],"about_ca_topic_score_codex":0.0011373818,"about_ca_topic_score_gemma":0.00062930165,"teacher_disagreement_score":0.0011373818,"about_ca_system_score_codex":0.00034936148,"about_ca_system_score_gemma":0.00009959241,"threshold_uncertainty_score":0.003384471},"labels":[],"label_agreement":null},{"id":"W1590668246","doi":"10.1086/367887","title":"<i>s</i>‐Process Nucleosynthesis in Asymptotic Giant Branch Stars: A Test for Stellar Evolution","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":216,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Nucleosynthesis; Physics; Asymptotic giant branch; Astrophysics; Metallicity; Stellar nucleosynthesis; Proton; Stellar evolution; Radiative transfer; s-process; Neutron star; Neutron; Stars; Nuclear physics; Quantum mechanics","score_opus":0.01170574172042325,"score_gpt":0.26165052635504615,"score_spread":0.2499447846346229,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1590668246","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99709773,0.000045074998,0.0015074804,0.000039073646,0.0000040972945,0.0000041629014,0.00005051787,0.00004495784,0.0012070652],"genre_scores_gemma":[0.9988651,0.000018680636,0.0008271497,0.000008149104,0.0000028410434,0.000004238842,0.00009124915,0.000018061757,0.00016438699],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999931,0.000021475546,0.0000034769885,0.000011781193,0.000014863777,0.00001736173],"domain_scores_gemma":[0.9994166,0.00032508356,0.00007236397,0.000044439686,0.00007519798,0.00006643398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032283424,0.00029815597,0.00025671968,0.00030251275,0.00026121995,0.00044261428,0.0005155757,0.0005068016,0.0011269753],"category_scores_gemma":[0.0014563452,0.00012180828,0.0005959575,0.00025528204,0.00037737,0.00025250937,0.00036356843,0.000240219,0.00014905435],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006761953,0.0001891032,0.11481014,0.00007019168,0.00011791115,0.00028818837,0.000104019906,0.8452761,0.02364442,0.007295339,0.00043041472,0.007097998],"study_design_scores_gemma":[0.00005036817,0.00021074928,0.017872667,0.0000070995393,0.000017210017,0.000055558383,0.000048917584,0.9747594,0.005091954,0.001661005,0.0002170617,0.0000080373475],"about_ca_topic_score_codex":0.0047435495,"about_ca_topic_score_gemma":0.0015800889,"teacher_disagreement_score":0.0047435495,"about_ca_system_score_codex":0.00046871504,"about_ca_system_score_gemma":0.00023498543,"threshold_uncertainty_score":0.009431899},"labels":[],"label_agreement":null},{"id":"W1590870017","doi":"10.1088/0004-637x/805/2/185","title":"AN AMMONIA SPECTRAL MAP OF THE L1495-B218 FILAMENTS IN THE TAURUS MOLECULAR CLOUD. I. PHYSICAL PROPERTIES OF FILAMENTS AND DENSE CORES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Molecular cloud; Virial theorem; Star formation; Spectral line; Protostar; Range (aeronautics); Spectral resolution; Gravitational collapse; Resolution (logic)","score_opus":0.017150441438906112,"score_gpt":0.24713845449514377,"score_spread":0.22998801305623764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1590870017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975199,0.00008468408,0.00024859334,0.000025322666,0.0000022630259,0.0000038299454,0.00047194667,0.00003687502,0.0016066736],"genre_scores_gemma":[0.9988232,0.000030368601,0.00046949746,0.000014813339,0.0000060079933,0.000003971091,0.000495673,0.0000051394386,0.00015130716],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997437,0.000001927359,0.0000013395343,0.000007911966,0.0000067078413,0.000007847798],"domain_scores_gemma":[0.9999045,0.000009965272,0.00003561177,0.000005768419,0.000011268809,0.0000328235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000033469933,0.00012741852,0.00011609656,0.0005635179,0.0002442859,0.000172013,0.00018355917,0.00026160802,0.001147718],"category_scores_gemma":[0.00010295525,0.00010436618,0.00014079755,0.0003395309,0.00012820253,0.00012837244,0.00019637054,0.00012409738,0.00017868637],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000695724,0.0001417542,0.4704224,0.000107318694,0.00009359307,0.0019289099,0.00043898853,0.002514878,0.49464324,0.0003123478,0.0019460513,0.026754824],"study_design_scores_gemma":[0.0000063275943,0.000028352038,0.9956857,0.0000073335614,0.000009513704,0.00017970602,0.000043277403,0.0019308854,0.0016303333,0.000043694687,0.00043207893,0.0000028395427],"about_ca_topic_score_codex":0.002685633,"about_ca_topic_score_gemma":0.00476839,"teacher_disagreement_score":0.002685633,"about_ca_system_score_codex":0.00018493755,"about_ca_system_score_gemma":0.00004844071,"threshold_uncertainty_score":0.0053399205},"labels":[],"label_agreement":null},{"id":"W1593813526","doi":"10.1088/0004-637x/808/1/35","title":"ROTATION OF GIANT STARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Angular momentum; Astrophysics; Specific relative angular momentum; Rotation (mathematics); Angular velocity; Dynamo theory; Stars; Moment of inertia; Total angular momentum quantum number; Angular momentum coupling; Magnetic field; Classical mechanics; Dynamo; Quantum mechanics; Geometry","score_opus":0.01849936762648699,"score_gpt":0.23790850434697075,"score_spread":0.21940913672048376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1593813526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99478334,0.00014475666,0.0011147701,0.00001859424,0.0000051555708,0.00000545099,0.0002526959,0.000037727656,0.003637551],"genre_scores_gemma":[0.99846137,0.000094179835,0.00031670686,0.0000070811725,0.0000032910198,0.000004901319,0.00034007913,0.000020869169,0.0007515811],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999726,0.0000037650057,0.0000011234985,0.000008855814,0.0000053699396,0.0000083142695],"domain_scores_gemma":[0.9999535,0.0000064738015,0.0000140647935,0.000008296416,0.0000069884754,0.000010647722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005152789,0.00020908893,0.0001601257,0.0001838275,0.00014563021,0.00033147514,0.000110757785,0.00021559001,0.0012110457],"category_scores_gemma":[0.00020353815,0.00008552941,0.00027275988,0.00018360032,0.00012709611,0.00010055106,0.00018214452,0.00009796871,0.0003563956],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009869189,0.00010459557,0.36528707,0.00026273716,0.0001707426,0.0006143625,0.0005505789,0.2484246,0.30972165,0.009579711,0.0021123616,0.062184695],"study_design_scores_gemma":[0.000083539984,0.0005655817,0.7342804,0.000038950348,0.00006886948,0.00072866963,0.00022325673,0.22729142,0.021590061,0.0029625224,0.012125034,0.00004156711],"about_ca_topic_score_codex":0.0018759131,"about_ca_topic_score_gemma":0.0018128416,"teacher_disagreement_score":0.0018759131,"about_ca_system_score_codex":0.00031308888,"about_ca_system_score_gemma":0.0001554591,"threshold_uncertainty_score":0.0040513277},"labels":[],"label_agreement":null},{"id":"W1594714851","doi":"10.1086/338126","title":"MASTER of the Cosmic Microwave Background Anisotropy Power Spectrum: A Fast Method for Statistical Analysis of Large and Complex Cosmic Microwave Background Data Sets","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":718,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cosmic microwave background; Anisotropy; Spectral density; COSMIC cancer database; Monte Carlo method; Cosmic background radiation; Microwave; Satellite","score_opus":0.04440580716695317,"score_gpt":0.3176308124305518,"score_spread":0.2732250052635986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1594714851","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.003925058,0.00015385267,0.99326247,0.000053598425,0.000024267554,0.000038935308,0.00063898886,0.0015735518,0.00032924954],"genre_scores_gemma":[0.05841179,0.00039004316,0.9340705,0.000075763455,0.00012988086,0.00032516342,0.0030120504,0.0009754828,0.0026093586],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990496,0.00027580428,0.00004886207,0.00016553048,0.00038759448,0.00007269535],"domain_scores_gemma":[0.9962845,0.0017633063,0.0003480549,0.00097079296,0.0005227883,0.00011051086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0030472497,0.00085556513,0.0010255123,0.0029712191,0.00044098528,0.00092102285,0.0013595718,0.00047472215,0.004073164],"category_scores_gemma":[0.01020261,0.00066745793,0.0010556695,0.0016710779,0.0007104361,0.0016111111,0.0015473961,0.0012358739,0.002440773],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026807692,0.00010926851,0.0118622985,0.00027104325,0.0004064176,0.00021271464,0.000247781,0.10599867,0.01801773,0.095258854,0.017275333,0.7500719],"study_design_scores_gemma":[0.00006328558,0.00010289755,0.008120069,0.000046502508,0.000056172925,0.00044805338,0.000050237297,0.83516437,0.014055822,0.10791066,0.033866324,0.000115608666],"about_ca_topic_score_codex":0.0017035608,"about_ca_topic_score_gemma":0.0020008532,"teacher_disagreement_score":0.004073164,"about_ca_system_score_codex":0.00035799237,"about_ca_system_score_gemma":0.001157875,"threshold_uncertainty_score":0.016115546},"labels":[],"label_agreement":null},{"id":"W1596024901","doi":"10.1086/317137","title":"Dissociative Recombination of H<sub>3</sub>O<sup>+</sup>, HD<sub>2</sub>O<sup>+</sup>, and D<sub>3</sub>O<sup>+</sup>","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Deuterium; Dissociative recombination; Isotopomers; Isotope; Fragmentation (computing); Ion; Branching fraction; Recombination; Atomic physics; Dissociation (chemistry); Molecule; Branching (polymer chemistry); Nuclear physics; Chemistry; Physical chemistry","score_opus":0.007395238314907845,"score_gpt":0.2002534300304694,"score_spread":0.19285819171556154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1596024901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99570256,0.00057770754,0.0018465953,0.000024192199,0.0000071476684,0.00001576455,0.000118596174,0.000022652508,0.0016847479],"genre_scores_gemma":[0.99777466,0.0002974359,0.0009517535,0.000026950227,0.0000052928945,0.000012008977,0.00020806673,0.000012376214,0.000711467],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998733,0.000013488455,0.000004500946,0.000047826885,0.000021900272,0.000038871596],"domain_scores_gemma":[0.9996489,0.00013987093,0.00011190218,0.000039739472,0.000026078762,0.000033441596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003555586,0.00048737953,0.0002844694,0.0003252299,0.00037427398,0.00027456772,0.00040505914,0.00024395052,0.002515721],"category_scores_gemma":[0.0003970891,0.00018551845,0.00021834967,0.00033382478,0.0003733798,0.0005156155,0.00053648447,0.000264616,0.0002558483],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013334824,0.0001826378,0.03804189,0.00028126122,0.00012512461,0.00042800306,0.000503334,0.002341318,0.9356364,0.0019037094,0.0003031227,0.01891959],"study_design_scores_gemma":[0.0000886684,0.0006821501,0.047962584,0.000011612963,0.00008629417,0.0005253116,0.000382981,0.006946242,0.939504,0.00095063646,0.00283138,0.000027993341],"about_ca_topic_score_codex":0.0007105691,"about_ca_topic_score_gemma":0.00080996926,"teacher_disagreement_score":0.002515721,"about_ca_system_score_codex":0.00023668217,"about_ca_system_score_gemma":0.00015278014,"threshold_uncertainty_score":0.008415937},"labels":[],"label_agreement":null},{"id":"W1598308997","doi":"10.1086/317234","title":"Shellflow. I. The Convergence of the Velocity Field at 6000 Kilometers per Second","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Peculiar velocity; Astrophysics; Cosmic microwave background; Galaxy; Amplitude; Redshift; Sky; Spurious relationship; Tully–Fisher relation; COSMIC cancer database; Extinction (optical mineralogy); Astronomy; Halo; Optics; Statistics","score_opus":0.005628125948876561,"score_gpt":0.19467282824876914,"score_spread":0.18904470229989256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1598308997","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22659726,0.00031415993,0.16623564,0.0003599171,0.00058237574,0.00049125776,0.34283143,0.16751744,0.0950706],"genre_scores_gemma":[0.34902275,0.00015964231,0.18452205,0.00014936134,0.00017589753,0.0004768413,0.42821568,0.018489487,0.01878833],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993691,0.000048842376,0.000048518054,0.00018654543,0.00025274907,0.00009423365],"domain_scores_gemma":[0.9982249,0.0003100262,0.000308282,0.00052432885,0.00046053718,0.00017186826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011283208,0.00066811277,0.00043568874,0.0020354677,0.0004246973,0.0010961499,0.0009870196,0.00030444056,0.02254885],"category_scores_gemma":[0.004442011,0.00041334072,0.0004930565,0.0013374456,0.00024945312,0.001281568,0.0012113648,0.00051398954,0.009507256],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022794036,0.00032779755,0.1447575,0.000411415,0.00020193636,0.00021190596,0.0008216981,0.016557036,0.012230219,0.017465867,0.42733243,0.37740284],"study_design_scores_gemma":[0.0005535333,0.00034908607,0.25478357,0.00018211232,0.000107915796,0.0007635267,0.00019188432,0.34441018,0.051077336,0.01225785,0.33516264,0.00016042186],"about_ca_topic_score_codex":0.012090676,"about_ca_topic_score_gemma":0.009185605,"teacher_disagreement_score":0.02254885,"about_ca_system_score_codex":0.00044258728,"about_ca_system_score_gemma":0.00066466734,"threshold_uncertainty_score":0.07543343},"labels":[],"label_agreement":null},{"id":"W1599170713","doi":"10.1088/0004-637x/805/1/36","title":"MEASUREMENTS OF E-MODE POLARIZATION AND TEMPERATURE-E-MODE CORRELATION IN THE COSMIC MICROWAVE BACKGROUND FROM 100 SQUARE DEGREES OF SPTPOL DATA","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Three-Speed Logic (Canada); Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Cosmic microwave background; Physics; Multipole expansion; Planck; Polarization (electrochemistry); Spectral density; Astrophysics; Computational physics; Cosmic background radiation; Spectral line; Optics; Anisotropy; Quantum mechanics; Statistics","score_opus":0.050907783159487914,"score_gpt":0.3078739705901936,"score_spread":0.2569661874307057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1599170713","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99249744,0.00005519387,0.0025200432,0.0000376933,0.000005792639,0.0000135653945,0.0024790613,0.00019697714,0.0021941375],"genre_scores_gemma":[0.990838,0.00009196696,0.002542603,0.00002421721,0.000026050273,0.00003099547,0.006133313,0.00008384227,0.00022888381],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962413,0.00004299255,0.000012746371,0.00011177282,0.00013750468,0.000070841976],"domain_scores_gemma":[0.9992693,0.00017271553,0.00018236725,0.00016042242,0.00010871839,0.00010646085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036896404,0.00053810125,0.00030290236,0.0014121542,0.00028624813,0.00051078247,0.00038570864,0.0002799888,0.0012105445],"category_scores_gemma":[0.0010466151,0.00031356802,0.00040915207,0.0015995542,0.00026348262,0.00037792852,0.0005911793,0.0005995755,0.0004711984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067197037,0.00019960252,0.8243836,0.00013052954,0.00034575458,0.0006963515,0.0005681206,0.014122719,0.11579154,0.0009119756,0.0025841834,0.039593555],"study_design_scores_gemma":[0.00002257767,0.00007206274,0.9752769,0.000008157344,0.000042679152,0.00028786252,0.000046903122,0.009135196,0.013078891,0.0001612734,0.001845892,0.00002173498],"about_ca_topic_score_codex":0.0017381153,"about_ca_topic_score_gemma":0.003433415,"teacher_disagreement_score":0.0017381153,"about_ca_system_score_codex":0.00033483803,"about_ca_system_score_gemma":0.00014350378,"threshold_uncertainty_score":0.004049659},"labels":[],"label_agreement":null},{"id":"W1602203789","doi":"10.1086/337965","title":"Limits to Interstellar C<sub>4</sub>and C<sub>5</sub>toward ζ Ophiuchi","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Interstellar cloud; Spectral line; Molecular cloud; High resolution; Spectral resolution; Abundance (ecology); Astronomy; Remote sensing; Stars","score_opus":0.009875603465141701,"score_gpt":0.2140948424174151,"score_spread":0.2042192389522734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1602203789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898431,0.0015408768,0.0015028854,0.00012078798,0.0000073188394,0.0000061518176,0.00012882202,0.00005085158,0.006799316],"genre_scores_gemma":[0.9983944,0.00028715812,0.0006344474,0.000058245205,0.000007539657,0.000005535656,0.00020088571,0.000004015149,0.00040770802],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978584,0.000017060183,0.000011491642,0.000057215864,0.00006908577,0.000059379796],"domain_scores_gemma":[0.99917656,0.00018510908,0.00029796857,0.00006873437,0.00014098952,0.00013052313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042785937,0.00039954166,0.00015130386,0.0009999793,0.0008135391,0.00078189344,0.000936174,0.00050924026,0.003473238],"category_scores_gemma":[0.00101134,0.0002366048,0.00012929308,0.00041667934,0.00066925766,0.00057331164,0.0009215662,0.00034338085,0.00047724726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078836596,0.00010027958,0.54141587,0.00032247519,0.00012999066,0.0007977301,0.0009917886,0.0021023143,0.39900064,0.009564812,0.00057692546,0.044208765],"study_design_scores_gemma":[0.000033197717,0.0002985354,0.8807472,0.00014751918,0.00012417824,0.0011419806,0.0014693278,0.0047581666,0.08668596,0.011667564,0.012881087,0.000045231292],"about_ca_topic_score_codex":0.005461481,"about_ca_topic_score_gemma":0.008503914,"teacher_disagreement_score":0.005461481,"about_ca_system_score_codex":0.00059838354,"about_ca_system_score_gemma":0.00033442775,"threshold_uncertainty_score":0.01161921},"labels":[],"label_agreement":null},{"id":"W1602726146","doi":"10.1088/0004-637x/806/2/247","title":"A MEASUREMENT OF GRAVITATIONAL LENSING OF THE COSMIC MICROWAVE BACKGROUND BY GALAXY CLUSTERS USING DATA FROM THE SOUTH POLE TELESCOPE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"SLAC National Accelerator Laboratory; McGill University; U.S. Department of Energy; Gordon and Betty Moore Foundation; Office of Science; Canada Research Chairs; National Aeronautics and Space Administration; University of Chicago; National Science Foundation","keywords":"Cosmic microwave background; Physics; Astrophysics; South Pole Telescope; Gravitational lens; Weak gravitational lensing; Galaxy; Galaxy cluster; Strong gravitational lensing; Telescope; Sigma; Astronomy; Redshift; Optics","score_opus":0.061028451613901594,"score_gpt":0.27844864003397307,"score_spread":0.2174201884200715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1602726146","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.871238,0.0009787087,0.110885635,0.00086037803,0.000038228318,0.00007786367,0.0037675502,0.00054499955,0.0116085755],"genre_scores_gemma":[0.96180487,0.0002714578,0.03567368,0.00005061428,0.000049360387,0.000021163414,0.0013110571,0.00003391995,0.0007838501],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959904,0.00007878317,0.000010872393,0.00010332837,0.00017684221,0.0000311484],"domain_scores_gemma":[0.99897134,0.00039615057,0.0003546913,0.00013388137,0.00007927262,0.00006471327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008548993,0.0004332297,0.00036670733,0.0016420034,0.0004973545,0.00063605513,0.0003751617,0.00043584904,0.000866733],"category_scores_gemma":[0.0025451195,0.00034288265,0.0004100073,0.00159772,0.00050294976,0.00055505655,0.00097074057,0.00057154364,0.00022177199],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002520264,0.00009088061,0.77246803,0.00026439107,0.00048656375,0.00044761726,0.0005621761,0.010528968,0.088513985,0.02320516,0.0019599393,0.10122028],"study_design_scores_gemma":[0.000032345804,0.00016583817,0.9361731,0.000025393598,0.00008821561,0.00053892325,0.00014983559,0.025824381,0.017896581,0.012009401,0.007028469,0.00006744377],"about_ca_topic_score_codex":0.0050005307,"about_ca_topic_score_gemma":0.010291535,"teacher_disagreement_score":0.0050005307,"about_ca_system_score_codex":0.00062561344,"about_ca_system_score_gemma":0.00030059688,"threshold_uncertainty_score":0.00994283},"labels":[],"label_agreement":null},{"id":"W1603661751","doi":"10.1088/0004-637x/805/2/156","title":"PSR J1930–1852: A PULSAR IN THE WIDEST KNOWN ORBIT AROUND ANOTHER NEUTRON STAR","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Neutron star; Orbital period; Binary pulsar; X-ray pulsar; Millisecond pulsar; Orbit (dynamics); Pulsar planet; Orbital elements","score_opus":0.027268713809996497,"score_gpt":0.3210147510189457,"score_spread":0.2937460372089492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1603661751","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967289,0.00013869256,0.00029087666,0.000095856565,0.00004680385,0.000011908427,0.0002695359,0.000032380958,0.0023849506],"genre_scores_gemma":[0.9974993,0.00005479288,0.0007535571,0.00016918538,0.000039294315,0.0000066288103,0.00085589435,0.000012379501,0.0006091147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989367,0.0000069925704,0.0000052591254,0.000039521423,0.000028545131,0.00002612782],"domain_scores_gemma":[0.9997719,0.00001081031,0.00005443591,0.000017775828,0.000017422788,0.00012762287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020954416,0.00035647192,0.00030012324,0.0005492242,0.0013544707,0.0004930421,0.00028202814,0.0004773708,0.001206257],"category_scores_gemma":[0.00022916275,0.00016668439,0.00017863474,0.00073900656,0.0004697342,0.00040153862,0.0007215955,0.00071649323,0.00054772303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008715877,0.0005212741,0.79036814,0.00017671632,0.00018967611,0.010182768,0.0016411328,0.00083399203,0.15405107,0.0029825885,0.008379844,0.029801194],"study_design_scores_gemma":[0.00005430253,0.00057129853,0.9733872,0.0000125598635,0.00004039048,0.0055395924,0.0007371577,0.0012085524,0.005363228,0.0006022531,0.012449061,0.000034412038],"about_ca_topic_score_codex":0.0041208365,"about_ca_topic_score_gemma":0.008946978,"teacher_disagreement_score":0.0041208365,"about_ca_system_score_codex":0.0004376161,"about_ca_system_score_gemma":0.00029045754,"threshold_uncertainty_score":0.008193672},"labels":[],"label_agreement":null},{"id":"W1606184554","doi":"10.1088/0004-637x/806/1/16","title":"CHAOS I. DIRECT CHEMICAL ABUNDANCES FOR ${\\rm H}\\;{\\rm II}$ REGIONS IN NGC 628","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":179,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Abundance (ecology); Spectrograph; Line (geometry); Dispersion (optics); Range (aeronautics); Interstellar medium; Spectral line; Spiral galaxy","score_opus":0.01655037082985185,"score_gpt":0.23725451870248213,"score_spread":0.22070414787263026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1606184554","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964965,0.000051899882,0.0002697994,0.000025378069,0.0000025351399,0.000004217876,0.001295273,0.000058184567,0.0017962174],"genre_scores_gemma":[0.9974094,0.000030169816,0.0006725829,0.000013728215,0.000005187997,0.0000075183175,0.0014843217,0.000018725614,0.00035838617],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998921,0.0000056394338,0.000008370203,0.000038652783,0.000033843247,0.000021414482],"domain_scores_gemma":[0.99974173,0.00002424641,0.00009886409,0.000032340402,0.00004553075,0.000057188412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010485308,0.00019593886,0.00013803897,0.0012435557,0.00024392748,0.00046346692,0.0001463566,0.0001612883,0.0010516014],"category_scores_gemma":[0.00056706945,0.00014029753,0.00019399976,0.0005886677,0.00022524792,0.00021002162,0.0005652377,0.00014919201,0.00032263913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013557363,0.00001598814,0.92342174,0.000029041677,0.00003784997,0.00010853474,0.00033102237,0.001179472,0.06373441,0.00062203757,0.00066083425,0.009723492],"study_design_scores_gemma":[0.000011931719,0.000036797945,0.989726,0.000010295372,0.000019326535,0.00013062861,0.00019377188,0.002545608,0.0049274447,0.0005110772,0.001876518,0.000010615267],"about_ca_topic_score_codex":0.0061770687,"about_ca_topic_score_gemma":0.014107888,"teacher_disagreement_score":0.0061770687,"about_ca_system_score_codex":0.00037982207,"about_ca_system_score_gemma":0.00014351185,"threshold_uncertainty_score":0.012282252},"labels":[],"label_agreement":null},{"id":"W1608416958","doi":"10.1086/376791","title":"Line Intensities and Molecular Opacities of the FeH<i>F</i><sup>4</sup>Δ<sub><i>i</i></sub>–<i>X</i><sup>4</sup>Δ<sub><i>i</i></sub>Transition","year":2003,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":198,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Line (geometry); Atomic physics; Opacity; Dipole; Brown dwarf; Einstein coefficients; Spectral line; Coupling constant; Stars; Astrophysics","score_opus":0.007588350919855247,"score_gpt":0.18612398022817203,"score_spread":0.1785356293083168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1608416958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9810922,0.00010578492,0.01088965,0.000030811487,0.0000063251186,0.000022614946,0.0015893221,0.00055211777,0.0057111937],"genre_scores_gemma":[0.98828644,0.00009159263,0.008702637,0.0000100766265,0.000005007734,0.00003846561,0.0015633821,0.000139476,0.001162895],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998807,0.000009663933,0.0000049849955,0.0000339439,0.00004865519,0.000022098611],"domain_scores_gemma":[0.9996371,0.00013452303,0.00007752285,0.000037851583,0.00009306149,0.000019816562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002283146,0.00032594227,0.00024308193,0.0011678181,0.00029542964,0.00036347122,0.0005841606,0.00044281114,0.0028314942],"category_scores_gemma":[0.00089879445,0.0004041982,0.00045177076,0.00095189747,0.00024985254,0.0006668656,0.00026666466,0.000470655,0.0005463635],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026566646,0.00017055849,0.11106402,0.00020594343,0.00015022494,0.0003028173,0.00043887383,0.74085796,0.06440563,0.008656497,0.0016294288,0.07185241],"study_design_scores_gemma":[0.00005521819,0.00013149403,0.12590477,0.000026564387,0.00006187094,0.0001713513,0.00012211243,0.7976241,0.06816469,0.0039802697,0.0036883727,0.000069298774],"about_ca_topic_score_codex":0.0024577535,"about_ca_topic_score_gemma":0.0027743776,"teacher_disagreement_score":0.0028314942,"about_ca_system_score_codex":0.0007147541,"about_ca_system_score_gemma":0.00022454778,"threshold_uncertainty_score":0.009472251},"labels":[],"label_agreement":null},{"id":"W1608695725","doi":"10.1088/0004-637x/760/2/145","title":"SECOND SEASON QUIET OBSERVATIONS: MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND POLARIZATION POWER SPECTRUM AT 95 GHz","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Fermilab; Science and Technology Facilities Council; Kavli Institute for Cosmological Physics, University of Chicago; Jet Propulsion Laboratory; Japan Society for the Promotion of Science; Office of Science; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Universitetet i Oslo; Northrop Grumman; National Science Foundation","keywords":"Cosmic microwave background; Physics; Spectral density; Polarization (electrochemistry); Spectral line; Gravitational wave; Astrophysics; Cosmic variance; Null (SQL); Computational physics; Optics; Statistics; Mathematics; Astronomy","score_opus":0.02686411129337303,"score_gpt":0.24835430679645254,"score_spread":0.22149019550307952,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1608695725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96657246,0.00023543513,0.010822857,0.000095350544,0.0000423638,0.000081487444,0.010252554,0.0006988338,0.011198682],"genre_scores_gemma":[0.9719885,0.000118344164,0.009223305,0.00009984585,0.00007690116,0.00009583162,0.016015388,0.00020444138,0.0021773644],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995127,0.000053933847,0.000017263892,0.00014139249,0.0001601206,0.000114570634],"domain_scores_gemma":[0.9994941,0.00006824867,0.0000887976,0.00012301924,0.0000786749,0.00014728715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071809546,0.00045854953,0.00038210498,0.001431706,0.0004009909,0.0007924447,0.00061177305,0.00031381924,0.002530305],"category_scores_gemma":[0.0006841169,0.00031353335,0.0004814549,0.0010353585,0.0002565748,0.0002754369,0.000708782,0.00058892724,0.00075582217],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001791383,0.00037411865,0.6674061,0.00022288912,0.00043870497,0.00056410127,0.0012033655,0.004780786,0.23123676,0.0035781872,0.012825544,0.075578086],"study_design_scores_gemma":[0.000097905235,0.00015031497,0.9682703,0.000015381307,0.00007996754,0.00020478328,0.000106475585,0.004362787,0.01697671,0.000286636,0.0094173,0.000031358326],"about_ca_topic_score_codex":0.004198582,"about_ca_topic_score_gemma":0.0066257953,"teacher_disagreement_score":0.004198582,"about_ca_system_score_codex":0.00031087123,"about_ca_system_score_gemma":0.00031506934,"threshold_uncertainty_score":0.008464694},"labels":[],"label_agreement":null},{"id":"W1611556424","doi":"10.1086/312499","title":"Emission Lines in the Spectrum of the [TSUP]3[/TSUP]H[CLC]e[/CLC] Star 3 Centauri A","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Multiplet; Astrophysics; Physics; Manganese; Emission spectrum; Astronomy; Spectral line; Chemistry","score_opus":0.008018589336206219,"score_gpt":0.2181405417605777,"score_spread":0.21012195242437148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1611556424","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958332,0.00007737028,0.00024879532,0.00004012742,0.0000058285605,0.0000028832726,0.000088424444,0.00007149455,0.0036319236],"genre_scores_gemma":[0.9988703,0.00003051846,0.00023367189,0.00004057543,0.0000046058535,0.0000028668626,0.00021824842,0.000016108268,0.000583071],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995255,0.0000028435586,0.0000015842916,0.00000856758,0.0000123294,0.000022175574],"domain_scores_gemma":[0.99986684,0.000013977413,0.000024434974,0.000012131471,0.00002700818,0.000055543962],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007283176,0.00013339978,0.000115738425,0.000537324,0.00042592624,0.00032304943,0.00016486803,0.00031427553,0.002016858],"category_scores_gemma":[0.00015972053,0.00010528148,0.00015492446,0.00047298538,0.0003087826,0.000119989934,0.00025106972,0.0002765099,0.00024171121],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006366612,0.000088324705,0.06836022,0.000086664935,0.00005529929,0.0012733673,0.00059748674,0.00062672613,0.9076036,0.0015907751,0.0015032722,0.017577652],"study_design_scores_gemma":[0.00004269182,0.00014508677,0.94351554,0.000017766191,0.00005053916,0.0008312851,0.00028913422,0.0017433966,0.049494047,0.000557476,0.0032845698,0.000028444036],"about_ca_topic_score_codex":0.002677563,"about_ca_topic_score_gemma":0.0038973636,"teacher_disagreement_score":0.002677563,"about_ca_system_score_codex":0.0002484728,"about_ca_system_score_gemma":0.00009282689,"threshold_uncertainty_score":0.0067471266},"labels":[],"label_agreement":null},{"id":"W1612374553","doi":"10.1088/0004-637x/705/1/766","title":"EVOLVING STARBURST MODELING OF FAR-INFRARED/SUBMILLIMETER/MILLIMETER LINE EMISSION. II. APPLICATION TO M 82","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Radiative transfer; Line (geometry); Photodissociation; Molecular cloud; Supernova; Star formation; Spectral line; Radiation pressure; Radiative cooling; Infrared","score_opus":0.012181251832892778,"score_gpt":0.2490221661231678,"score_spread":0.236840914290275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1612374553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8475879,0.0005725669,0.13908039,0.00034523266,0.0000517787,0.00007375137,0.0008211738,0.00089296163,0.01057426],"genre_scores_gemma":[0.9710397,0.00029623267,0.024352811,0.00007019213,0.000023652019,0.000058257065,0.00038091553,0.00017779546,0.0036005026],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994636,0.000011077239,0.0000027922622,0.000017567058,0.000011272054,0.000010878329],"domain_scores_gemma":[0.9998342,0.00005566262,0.000036727542,0.000018555029,0.000026950127,0.000027889486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015627146,0.0004803547,0.0003094126,0.00016330236,0.00027301302,0.00059980823,0.0010415546,0.00082567876,0.0011464544],"category_scores_gemma":[0.0006278002,0.00026904015,0.0005824832,0.00025047507,0.00021613234,0.0004171688,0.00049229566,0.00040478545,0.0002651931],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030003912,0.000028126806,0.006340097,0.000022557286,0.00002559798,0.00018568012,0.00006410108,0.9844242,0.002770371,0.0017570624,0.00029792107,0.0040544225],"study_design_scores_gemma":[0.000005657192,0.000009404699,0.0011925753,0.0000018352416,0.000005311532,0.000027424638,0.000013642736,0.9974947,0.00032702624,0.00049452274,0.00042564512,0.0000023360637],"about_ca_topic_score_codex":0.021374593,"about_ca_topic_score_gemma":0.009620113,"teacher_disagreement_score":0.021374593,"about_ca_system_score_codex":0.00068793964,"about_ca_system_score_gemma":0.00038594435,"threshold_uncertainty_score":0.042500317},"labels":[],"label_agreement":null},{"id":"W1614678536","doi":"10.1088/0004-637x/775/2/134","title":"THE AGES OF 55 GLOBULAR CLUSTERS AS DETERMINED USING AN IMPROVED $\\Delta V^{\\rm HB}_{\\rm TO}$ METHOD ALONG WITH COLOR-MAGNITUDE DIAGRAM CONSTRAINTS, AND THEIR IMPLICATIONS FOR BROADER ISSUES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":494,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Subgiant; Physics; Globular cluster; Astrophysics; Metallicity; Horizontal branch; Red-giant branch; Stars; Photometry (optics); Hubble space telescope; Absolute magnitude; Hertzsprung–Russell diagram; Star cluster; Stellar evolution","score_opus":0.017317938177450462,"score_gpt":0.28814642287359793,"score_spread":0.27082848469614745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1614678536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9813953,0.0006872992,0.0056494866,0.000029356619,0.000027140157,0.000028236507,0.007612963,0.00016563089,0.0044045197],"genre_scores_gemma":[0.9820893,0.00032342697,0.0070600347,0.000016721893,0.00000994414,0.000018775592,0.009366406,0.000025587924,0.0010898086],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99941707,0.000056772406,0.000054844746,0.000297547,0.0000860103,0.000087752385],"domain_scores_gemma":[0.9987418,0.00031116002,0.00020917608,0.0003141965,0.0003043532,0.00011931778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014488443,0.00042938322,0.0003873308,0.0027532668,0.0008686723,0.00086059386,0.0005415964,0.00035781116,0.0015096499],"category_scores_gemma":[0.0021367306,0.00018576079,0.0006334984,0.0018512154,0.0005156128,0.00042385646,0.0007605945,0.0003186411,0.00094153715],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043145087,0.000036088233,0.9375551,0.00013488847,0.00032849418,0.00016088766,0.00091173715,0.0079404805,0.010118383,0.0031117122,0.0019702662,0.037300494],"study_design_scores_gemma":[0.0000190044,0.00008553901,0.9734389,0.000032631182,0.00019423403,0.00017336615,0.00033783424,0.0071249516,0.007090615,0.0007659153,0.010700794,0.000036180103],"about_ca_topic_score_codex":0.03514744,"about_ca_topic_score_gemma":0.039408326,"teacher_disagreement_score":0.03514744,"about_ca_system_score_codex":0.0014458968,"about_ca_system_score_gemma":0.0006659736,"threshold_uncertainty_score":0.06988567},"labels":[],"label_agreement":null},{"id":"W1617077345","doi":"10.1088/0004-637x/809/1/67","title":"DISCOVERY AND FOLLOW-UP OF ROTATING RADIO TRANSIENTS WITH THE GREEN BANK AND LOFAR TELESCOPES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Research Chairs; National Radio Astronomy Observatory; Compute Canada; Associated Universities; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Pulsar; LOFAR; Green Bank Telescope; Dispersion (optics); Radio telescope; Low frequency; Telescope","score_opus":0.013542908883786696,"score_gpt":0.2748305555621667,"score_spread":0.26128764667838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1617077345","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969337,0.00016301947,0.0014116592,0.00004484233,0.0000082776905,0.000011061541,0.00039998937,0.00006109063,0.00096636015],"genre_scores_gemma":[0.99584717,0.00007524284,0.0028050833,0.000043293418,0.000013671086,0.000014090627,0.00077057554,0.000020497773,0.00041033936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975544,0.00003091797,0.000012574186,0.000073040625,0.00005669709,0.0000712404],"domain_scores_gemma":[0.9983454,0.00026650785,0.00065722404,0.0001949616,0.00020109664,0.00033484874],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007508626,0.00018398183,0.0003132471,0.0017819343,0.00050126575,0.0006157749,0.00032866886,0.00018010853,0.0007590229],"category_scores_gemma":[0.0013475996,0.00021967506,0.00018081073,0.0013168168,0.00029370977,0.0002555202,0.00060208724,0.00037492014,0.00035339769],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016902236,0.00004845888,0.9457672,0.000035128967,0.00008315205,0.00036298425,0.00057568087,0.0010993634,0.027952943,0.00049404165,0.0009707702,0.022441259],"study_design_scores_gemma":[0.000009102098,0.000035541736,0.99578,0.0000067868045,0.00002157912,0.00015574529,0.000076488715,0.0013205023,0.0013243471,0.000062882216,0.0011982177,0.000008878742],"about_ca_topic_score_codex":0.0070261364,"about_ca_topic_score_gemma":0.01483335,"teacher_disagreement_score":0.0070261364,"about_ca_system_score_codex":0.00054854195,"about_ca_system_score_gemma":0.0003500404,"threshold_uncertainty_score":0.013970494},"labels":[],"label_agreement":null},{"id":"W1617877108","doi":"10.1086/319104","title":"The Metallicity of 0.5 &lt; [CLC][ITAL]z[/ITAL][/CLC] &lt; 1 Field Galaxies","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Metallicity; Galaxy; Redshift; Peculiar galaxy; Astronomy; Luminous infrared galaxy; Galaxy group","score_opus":0.007969939676678427,"score_gpt":0.21436630548580776,"score_spread":0.20639636580912935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1617877108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984187,0.000057434714,0.00006768508,0.0000102462145,9.32775e-7,0.0000029143812,0.0004474501,0.0000121510175,0.0009824957],"genre_scores_gemma":[0.99874204,0.000023748818,0.000115024,0.0000074618447,0.0000028031009,0.000001894471,0.00065996597,0.0000022646275,0.00044479233],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999874,0.000009411124,0.000005875049,0.000031524956,0.000019917308,0.000059292503],"domain_scores_gemma":[0.99951196,0.000053572,0.00017581739,0.000054949116,0.00010717327,0.00009656957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033577593,0.00017991939,0.00014650838,0.0017010642,0.00034066098,0.00046292334,0.00027446513,0.00013077304,0.0022113621],"category_scores_gemma":[0.00053150684,0.000102617385,0.000103770464,0.000681652,0.00037087366,0.00026410967,0.00020237493,0.00012838261,0.0005542656],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008932887,0.000024157294,0.98514646,0.00001220603,0.000014289101,0.00005355391,0.0001832488,0.00012168333,0.0064982404,0.0002604302,0.0002886903,0.007307837],"study_design_scores_gemma":[0.0000026673463,0.00001464396,0.99899966,0.000002232919,0.000004985312,0.000028863084,0.000034200526,0.00009880333,0.0004935225,0.000026904865,0.00029211267,0.0000014120902],"about_ca_topic_score_codex":0.016606832,"about_ca_topic_score_gemma":0.020772042,"teacher_disagreement_score":0.016606832,"about_ca_system_score_codex":0.00069178705,"about_ca_system_score_gemma":0.00011942171,"threshold_uncertainty_score":0.033020377},"labels":[],"label_agreement":null},{"id":"W1618367684","doi":"10.1086/308310","title":"The<i>Hubble Space Telescope</i>Key Project on the Extragalactic Distance Scale. XXVII. A Derivation of the Hubble Constant Using the Fundamental Plane and \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $D_{n}$ \\end{document} ‐σ Relations in Leo I, Virgo, and Fornax","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Cepheid variable; Physics; Fundamental plane (elliptical galaxies); Hubble's law; Cosmic microwave background; Tully–Fisher relation; Astrophysics; Cosmic distance ladder; Redshift; Galaxy; Galaxy cluster; Galaxy formation and evolution; Optics; Stars","score_opus":0.013649449290070741,"score_gpt":0.24111415347077833,"score_spread":0.22746470418070758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1618367684","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.010273663,0.026090953,0.11979065,0.011330399,0.008749823,0.0003949057,0.050025247,0.010761061,0.76258326],"genre_scores_gemma":[0.10429319,0.016516842,0.12558492,0.0015635721,0.0034641805,0.0007106328,0.07869981,0.01198022,0.65718675],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998128,0.000021679947,0.000008320825,0.00003263422,0.0001016984,0.000022977645],"domain_scores_gemma":[0.9997235,0.000040531428,0.000041938045,0.00007910747,0.000080121,0.00003477396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000598115,0.00097034016,0.00039147955,0.0014406665,0.00068506517,0.0019622142,0.0011466492,0.0008173831,0.082847945],"category_scores_gemma":[0.0011419371,0.0004675711,0.00075957034,0.0023251062,0.00047948913,0.0016254784,0.00091253023,0.0025870686,0.054492105],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054603526,0.000033983022,0.0006878249,0.0002826416,0.000023455363,0.00007197033,0.00012319878,0.00067704596,0.0024467579,0.15907672,0.7069081,0.12961368],"study_design_scores_gemma":[0.00003220363,0.000017417426,0.0071544,0.0000931419,0.000011337952,0.000081019454,0.0000329559,0.0010214142,0.0019675088,0.05010827,0.939457,0.00002333694],"about_ca_topic_score_codex":0.0094871605,"about_ca_topic_score_gemma":0.007873126,"teacher_disagreement_score":0.082847945,"about_ca_system_score_codex":0.0021923273,"about_ca_system_score_gemma":0.0006266467,"threshold_uncertainty_score":0.27715403},"labels":[],"label_agreement":null},{"id":"W1618529732","doi":"10.1086/317334","title":"A Lack of Planets in 47 Tucanae from a [ITAL]Hubble Space Telescope[/ITAL] Search","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":291,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Calgary","funders":"","keywords":"Physics; Planet; Astronomy; Astrophysics; Globular cluster; Hot Jupiter; Terrestrial planet; Stars; Solar System; Exoplanet; Planetary system","score_opus":0.01862783356840103,"score_gpt":0.25018974576363207,"score_spread":0.23156191219523103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1618529732","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983236,0.000063743886,0.00007350792,0.000023485136,0.0000022031766,0.0000026086361,0.000674963,0.000014145754,0.00082168455],"genre_scores_gemma":[0.99554896,0.000048669972,0.00021892895,0.000026561198,0.0000043910004,0.000003967071,0.0036230665,0.0000069944235,0.0005184576],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999777,0.000012011763,0.000007808008,0.00004729579,0.000056391367,0.00009946005],"domain_scores_gemma":[0.9995709,0.000056662568,0.000103810125,0.00006472327,0.00009319671,0.000110718815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019267175,0.00016106898,0.00037019685,0.00096028013,0.0011832977,0.0006335588,0.0004002881,0.00035486915,0.002292775],"category_scores_gemma":[0.00051277305,0.00008572636,0.00017792963,0.0014343447,0.00036127167,0.00017629442,0.000390032,0.00021873286,0.00032955807],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004378128,0.00009066611,0.95969504,0.000048171514,0.00016638497,0.00060498196,0.00068455184,0.0009569325,0.012328568,0.00042970563,0.0024218983,0.022135163],"study_design_scores_gemma":[0.000008973765,0.000043785618,0.99197024,0.0000070999763,0.000057659876,0.0003393927,0.00029740107,0.00083233137,0.0021128864,0.00007348224,0.0042491877,0.0000076144247],"about_ca_topic_score_codex":0.12194441,"about_ca_topic_score_gemma":0.2037668,"teacher_disagreement_score":0.12194441,"about_ca_system_score_codex":0.0006742693,"about_ca_system_score_gemma":0.00087008224,"threshold_uncertainty_score":0.24246925},"labels":[],"label_agreement":null},{"id":"W1620589376","doi":"10.1086/498561","title":"Observations of the Circumstellar Water \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $1_{10}arrow 1_{01}$ \\end{document} and Ammonia \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $1_{0}arrow 0_{0}$ \\end{document} Lines in IRC +10216 by the<i>Odin</i>Satellite","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geology and Paleoclimatology Research","field":"Earth and Planetary Sciences","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Line (geometry); Astrophysics; Carbon star; Infrared; Spectral line; Atomic physics; Stars; Astronomy","score_opus":0.013980839003993857,"score_gpt":0.2278158215951625,"score_spread":0.21383498259116865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1620589376","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22237787,0.000812626,0.01091347,0.0017473504,0.0005058193,0.00032312467,0.07080579,0.013765796,0.67874825],"genre_scores_gemma":[0.5162366,0.0015841317,0.013209997,0.00078123045,0.00017358815,0.00015835375,0.06511,0.0074497955,0.39529628],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.999931,0.0000024174485,0.000002276015,0.000013350043,0.000036979978,0.000014028978],"domain_scores_gemma":[0.9999236,0.000010569281,0.000007658278,0.00001914514,0.00002244486,0.00001659513],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00009890542,0.00027304192,0.00010620644,0.00043636622,0.00038724425,0.0007757565,0.0003339142,0.00037963223,0.089254424],"category_scores_gemma":[0.00024680895,0.00020159995,0.00024377635,0.0007716292,0.0001497877,0.0004928645,0.00034953724,0.00039930484,0.03378035],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059209316,0.00015667832,0.017204255,0.0006821684,0.000066165056,0.0008947599,0.0005699516,0.0013764742,0.3156852,0.0037129128,0.38233668,0.27672264],"study_design_scores_gemma":[0.000073332965,0.0000920557,0.08079725,0.00007670445,0.000040845454,0.00015745246,0.00029772148,0.0019666578,0.08890252,0.0010188932,0.82654625,0.00003036361],"about_ca_topic_score_codex":0.009921638,"about_ca_topic_score_gemma":0.017082755,"teacher_disagreement_score":0.91074556,"about_ca_system_score_codex":0.00053970906,"about_ca_system_score_gemma":0.00026674962,"threshold_uncertainty_score":0.29858577},"labels":[],"label_agreement":null},{"id":"W1623609435","doi":"10.1088/0004-637x/807/1/16","title":"A MILLISECOND INTERFEROMETRIC SEARCH FOR FAST RADIO BURSTS WITH THE VERY LARGE ARRAY","year":2015,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Millisecond; Fast radio burst; Millisecond pulsar; Sky; Brightness; Attenuation; Pulsar; Optics; Astronomy; Neutron star","score_opus":0.02334297130097749,"score_gpt":0.32297250292969465,"score_spread":0.29962953162871714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1623609435","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9699718,0.0013805832,0.02086984,0.0003245627,0.00008985738,0.00005103987,0.00093270536,0.00040893763,0.005970598],"genre_scores_gemma":[0.9728842,0.00026788306,0.024273567,0.00018757426,0.00010684429,0.000029909703,0.0014225602,0.0000484161,0.00077912555],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999637,0.00005276102,0.000016016658,0.00010019169,0.00011672903,0.00007731102],"domain_scores_gemma":[0.99914885,0.00023013612,0.00023265887,0.00010813732,0.00010589488,0.00017439044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005899421,0.00019764373,0.00019526597,0.0012516177,0.00041773266,0.00069197663,0.00043374556,0.00040554575,0.0006599312],"category_scores_gemma":[0.0012483544,0.00023039707,0.00022699856,0.00064420357,0.00017890579,0.00046524545,0.00058872404,0.00039361423,0.0002876683],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038123733,0.00018406157,0.63160914,0.00012856076,0.0001713618,0.00083081855,0.0005469836,0.0017293754,0.13035004,0.0015271563,0.0037386853,0.22880252],"study_design_scores_gemma":[0.000054209202,0.0009504204,0.93075645,0.000044087745,0.0001657342,0.005166765,0.00029841543,0.013150444,0.026353488,0.0011200131,0.021852925,0.00008699604],"about_ca_topic_score_codex":0.000887821,"about_ca_topic_score_gemma":0.0018390616,"teacher_disagreement_score":0.0012516177,"about_ca_system_score_codex":0.00021918798,"about_ca_system_score_gemma":0.00022875257,"threshold_uncertainty_score":0.0031199455},"labels":[],"label_agreement":null},{"id":"W1626761104","doi":"10.1088/0004-637x/809/2/108","title":"SPIN AND MAGNETISM OF WHITE DWARFS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Dynamo; Astrophysics; Magnetic helicity; Magnetism; Dynamo theory; White dwarf; Magnetic field; Angular momentum; Condensed matter physics; Stars; Classical mechanics; Quantum mechanics","score_opus":0.014066867308527587,"score_gpt":0.23065361919469596,"score_spread":0.21658675188616838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1626761104","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99575436,0.0009823552,0.00009746319,0.000024267056,0.0000074560867,0.0000018595863,0.0000741328,0.0000034211282,0.0030545883],"genre_scores_gemma":[0.9982383,0.00036141742,0.00005105138,0.000013110028,0.0000103427765,9.53306e-7,0.000102115664,0.0000015098437,0.0012211961],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995935,0.000007997831,0.0000021796898,0.000010523242,0.000008853356,0.000011212289],"domain_scores_gemma":[0.9998996,0.000010326244,0.000035080095,0.0000054915804,0.000016219565,0.000033316046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001043049,0.00008965403,0.00011659114,0.00040512247,0.00021269766,0.00047086435,0.00007388647,0.000110339286,0.0004941548],"category_scores_gemma":[0.00020761073,0.00004343743,0.00006795456,0.00021069634,0.00027151188,0.0001331286,0.00021146938,0.0000912596,0.00013620897],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019135292,0.00011441744,0.65799356,0.0001345417,0.00009840765,0.00078579324,0.0018798185,0.00053826737,0.2898889,0.0046831425,0.0007081906,0.04126142],"study_design_scores_gemma":[0.000011816842,0.00029470577,0.9851509,0.000011369284,0.000019744697,0.00057211006,0.0006637539,0.0003629213,0.007275295,0.0009888995,0.004640245,0.0000082799725],"about_ca_topic_score_codex":0.002726209,"about_ca_topic_score_gemma":0.0035219805,"teacher_disagreement_score":0.002726209,"about_ca_system_score_codex":0.00027345744,"about_ca_system_score_gemma":0.00009604753,"threshold_uncertainty_score":0.005420685},"labels":[],"label_agreement":null},{"id":"W1630925398","doi":"10.1088/0004-637x/808/2/132","title":"CHEMICAL CARTOGRAPHY WITH APOGEE: METALLICITY DISTRIBUTION FUNCTIONS AND THE CHEMICAL STRUCTURE OF THE MILKY WAY DISK","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":613,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Ministerio de Economía y Competitividad; York University; Science and Technology Facilities Council; Carnegie Mellon University; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; University of Arizona; Office of Science; Alfred P. Sloan Foundation; University of Washington; Princeton University; College of Engineering, Michigan State University; Johns Hopkins University; University of Michigan; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Brookhaven National Laboratory; U.S. Department of Energy; W. M. Keck Foundation; National Science Foundation","keywords":"Milky Way; Metallicity; Stars; RADIUS; Thick disk; Star count; Stellar kinematics; Distribution (mathematics)","score_opus":0.006599589702912307,"score_gpt":0.19151686924852096,"score_spread":0.18491727954560866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1630925398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998166,0.00007563868,0.00020103213,0.000018479359,0.0000011339894,0.0000035053201,0.0009997606,0.000029918683,0.000504508],"genre_scores_gemma":[0.99712986,0.00006103795,0.0006442268,0.000010066495,0.0000049144182,0.0000064039764,0.0017037254,0.000013005883,0.00042690514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999859,0.000023052984,0.000012353809,0.000051635132,0.00002934311,0.00002454715],"domain_scores_gemma":[0.9986658,0.00026058868,0.0005820889,0.00020551683,0.00013074013,0.00015536025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023461472,0.00018724153,0.00027892517,0.0033263527,0.00022106222,0.00082743587,0.00022196639,0.00023624368,0.0019273778],"category_scores_gemma":[0.0011136476,0.00013649513,0.00024665086,0.0020251444,0.00026714613,0.00043784082,0.0007943775,0.00018962663,0.000670149],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048261918,0.000009802722,0.9914233,0.000012796797,0.000054644697,0.000041035873,0.0002499052,0.0002631188,0.0020406318,0.00009858697,0.00032352316,0.005434515],"study_design_scores_gemma":[0.0000018936538,0.000007588968,0.9987721,0.0000016269594,0.000007696577,0.00006084207,0.000076063465,0.0003455855,0.00018905089,0.00005003677,0.00048509933,0.000002502681],"about_ca_topic_score_codex":0.008109774,"about_ca_topic_score_gemma":0.01163874,"teacher_disagreement_score":0.008109774,"about_ca_system_score_codex":0.00017188495,"about_ca_system_score_gemma":0.000116827505,"threshold_uncertainty_score":0.016125143},"labels":[],"label_agreement":null},{"id":"W1637512816","doi":"10.1086/427066","title":"RCS 043938-2904.9: A New Rich Cluster of Galaxies at [FORMULA][F]z=0.951[/F][/FORMULA]","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Redshift; Astrophysics; Physics; Cluster (spacecraft); Galaxy; Galaxy cluster; Spectroscopy; Brightest cluster galaxy; Magnitude (astronomy); Astronomy","score_opus":0.007540992606335592,"score_gpt":0.2127935868368398,"score_spread":0.2052525942305042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1637512816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8778893,0.0010693002,0.004347983,0.0026794516,0.0005586486,0.00029243328,0.024120446,0.0042416574,0.084800795],"genre_scores_gemma":[0.8601601,0.0003170328,0.0066390885,0.0011176692,0.000574546,0.00011872222,0.03502049,0.00081158144,0.09524082],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997093,0.00002307188,0.0000136449935,0.000089296154,0.00008562275,0.000079184625],"domain_scores_gemma":[0.9993149,0.000031216972,0.00009084887,0.00009003087,0.00009220731,0.00038073334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033235198,0.00043570055,0.0006098726,0.0030999887,0.0019708346,0.0011612052,0.0011998203,0.0007092776,0.04254378],"category_scores_gemma":[0.000466169,0.00026857347,0.00044372637,0.002610777,0.00070152595,0.0006123433,0.0015917562,0.0007986413,0.01884598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025539978,0.0010705349,0.47267455,0.0004548142,0.00029327816,0.010717781,0.0037365966,0.00053985335,0.07162782,0.023662547,0.23524956,0.17741872],"study_design_scores_gemma":[0.00020272554,0.0002881014,0.746118,0.00004931119,0.000111900175,0.009812432,0.0013364061,0.00067543035,0.004399047,0.002846601,0.23409119,0.00006884352],"about_ca_topic_score_codex":0.014822628,"about_ca_topic_score_gemma":0.019414512,"teacher_disagreement_score":0.04254378,"about_ca_system_score_codex":0.0007239001,"about_ca_system_score_gemma":0.0007025352,"threshold_uncertainty_score":0.14232308},"labels":[],"label_agreement":null},{"id":"W1638974416","doi":"10.1088/0004-637x/735/1/40","title":"THE INFLUENCE OF UNCERTAINTIES IN THE<sup>15</sup>O(α, γ)<sup>19</sup>Ne REACTION RATE ON MODELS OF TYPE I X-RAY BURSTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF","funders":"","keywords":"Nucleosynthesis; Reaction rate; Monte Carlo method; Type (biology); Neutron; Neutron star","score_opus":0.022211035299149938,"score_gpt":0.23684754651528336,"score_spread":0.21463651121613342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1638974416","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9736205,0.0005187026,0.022220904,0.000120766046,0.000022548438,0.000026475776,0.0001458386,0.00013219898,0.003192118],"genre_scores_gemma":[0.9962459,0.00016871082,0.0031789665,0.000018122992,0.000011962504,0.000023730661,0.000083705934,0.00005775767,0.00021116302],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99919766,0.00043503818,0.00005485969,0.0001162214,0.00013412297,0.00006203419],"domain_scores_gemma":[0.9853119,0.012036471,0.0010522617,0.00090161513,0.00047789773,0.00021970447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00265674,0.0008949413,0.0005878398,0.0004900332,0.0005029416,0.001216538,0.0013537123,0.0007188421,0.0006664822],"category_scores_gemma":[0.014273653,0.0005245014,0.0010019309,0.00034567362,0.00067335996,0.000869275,0.00068304036,0.0006102799,0.00017427177],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001795915,0.00002141203,0.010423068,0.000018263923,0.00005367277,0.00007072614,0.000023839988,0.98464555,0.0015065217,0.0014910868,0.000043953118,0.0015223798],"study_design_scores_gemma":[0.000024811856,0.000091684065,0.0032492378,0.000010692249,0.00005777304,0.000053076124,0.00001806093,0.99144906,0.0034811015,0.001380959,0.00016076327,0.000022795799],"about_ca_topic_score_codex":0.006263658,"about_ca_topic_score_gemma":0.0031086756,"teacher_disagreement_score":0.006263658,"about_ca_system_score_codex":0.001204299,"about_ca_system_score_gemma":0.00044177272,"threshold_uncertainty_score":0.0140503645},"labels":[],"label_agreement":null},{"id":"W1640583519","doi":"10.1088/0004-637x/805/2/157","title":"THE BOLOCAM GALACTIC PLANE SURVEY. XIII. PHYSICAL PROPERTIES AND MASS FUNCTIONS OF DENSE MOLECULAR CLOUD STRUCTURES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galactic plane; Molecular cloud; High mass; Galaxy; Stellar population; Initial mass function; Formalism (music); Population; Interstellar medium; Spectral index","score_opus":0.02265322681318856,"score_gpt":0.23448385962147403,"score_spread":0.21183063280828546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1640583519","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.37446895,0.0031619833,0.0014155358,0.0005826411,0.00008087647,0.0002278385,0.59392005,0.00060670055,0.025535459],"genre_scores_gemma":[0.43965915,0.0019507704,0.0037978117,0.00017123343,0.00011329546,0.00022663023,0.544783,0.00011576095,0.009182381],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987936,0.0000130977105,0.000011440533,0.000028035445,0.000042658903,0.000025414534],"domain_scores_gemma":[0.9993765,0.000034474077,0.00027871787,0.000055504755,0.00014467872,0.00011015671],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028054163,0.00047112297,0.00021940943,0.00575931,0.00021627024,0.0006561883,0.0003958124,0.00021902546,0.0041493834],"category_scores_gemma":[0.000809514,0.00016300182,0.00024122337,0.0047813267,0.0001131039,0.00027970385,0.00055547996,0.0003468531,0.0033180239],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012832048,0.00004557426,0.88909596,0.00011840887,0.0001479026,0.00012017815,0.00019541173,0.0005286006,0.0013945915,0.000681283,0.07364392,0.033899892],"study_design_scores_gemma":[0.000010477204,0.0000067269957,0.98841184,0.000014281974,0.00000899322,0.00004136869,0.000038269856,0.00019142084,0.0001099163,0.00005829377,0.0111061465,0.0000022518088],"about_ca_topic_score_codex":0.0708781,"about_ca_topic_score_gemma":0.060430992,"teacher_disagreement_score":0.0708781,"about_ca_system_score_codex":0.0008250303,"about_ca_system_score_gemma":0.00032424385,"threshold_uncertainty_score":0.14093107},"labels":[],"label_agreement":null},{"id":"W1644684475","doi":"10.1086/507083","title":"The Importance of<sup>15</sup>O(α,γ)<sup>19</sup>Ne to X‐Ray Bursts and Superbursts","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF","funders":"","keywords":"Physics; Neutron star; Thermonuclear fusion; Nuclear reaction; Nucleosynthesis; Reaction rate; Nuclear astrophysics; Astrophysics; Resonance (particle physics); Nuclear physics; Stars; Neutron; Atomic physics; Plasma; Chemistry","score_opus":0.00733266875356028,"score_gpt":0.22290683804633474,"score_spread":0.21557416929277445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1644684475","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9810596,0.0018265577,0.0025911012,0.00042463955,0.000047986145,0.000024124785,0.00045380343,0.000082817955,0.0134894075],"genre_scores_gemma":[0.9974376,0.00074953766,0.00041031427,0.000105723186,0.000046212066,0.0000068868085,0.00015981379,0.000020638163,0.0010632557],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99967706,0.000088940826,0.000035964244,0.000087104265,0.00006278428,0.000048174476],"domain_scores_gemma":[0.99647224,0.0017911335,0.000958387,0.0004297132,0.00016125543,0.00018735274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061200926,0.00028629453,0.00025927095,0.0005683072,0.00023332554,0.0012087276,0.0003575236,0.0003891833,0.0036763947],"category_scores_gemma":[0.003750447,0.0002294367,0.00018714907,0.0003981603,0.00058947055,0.00065602135,0.0005122642,0.0003407664,0.00035435884],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024696107,0.00014817111,0.68085086,0.00070454704,0.00019794065,0.00079944596,0.0004154825,0.017989656,0.19791362,0.010385547,0.0008640368,0.08726104],"study_design_scores_gemma":[0.000019009387,0.00024661832,0.9230031,0.00007331935,0.00010338128,0.0013837565,0.00027624556,0.006923836,0.05630921,0.0049936865,0.006646372,0.000021496213],"about_ca_topic_score_codex":0.0013875543,"about_ca_topic_score_gemma":0.0010861165,"teacher_disagreement_score":0.0036763947,"about_ca_system_score_codex":0.0002668198,"about_ca_system_score_gemma":0.000101566766,"threshold_uncertainty_score":0.012298703},"labels":[],"label_agreement":null},{"id":"W1648277683","doi":"10.1088/0004-637x/809/2/153","title":"GHIGLS: H I MAPPING AT INTERMEDIATE GALACTIC LATITUDE USING THE GREEN BANK TELESCOPE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université Laval; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Spectral line; Interstellar medium; Green Bank Telescope; Line (geometry); Ecliptic; Exponent; Latitude; Scaling","score_opus":0.0362614090709555,"score_gpt":0.2682000307783053,"score_spread":0.2319386217073498,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1648277683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.63242126,0.0014577988,0.081110366,0.0008808222,0.00018753124,0.0006137532,0.18936862,0.028578935,0.065380946],"genre_scores_gemma":[0.65261155,0.00057381333,0.14649656,0.00055195845,0.0001283354,0.0004409206,0.18492903,0.0020280802,0.012239727],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974936,0.000029500576,0.0000056574318,0.000056761066,0.00008973735,0.00006907739],"domain_scores_gemma":[0.999694,0.000022801212,0.000041120733,0.00006213198,0.00005845477,0.000121533136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005954343,0.00048071382,0.00030494106,0.001503031,0.00042440894,0.00072325015,0.0006839396,0.0003169215,0.006228755],"category_scores_gemma":[0.0004910877,0.0003063841,0.0003384823,0.001378761,0.00024777467,0.00047928697,0.0010776303,0.0003776444,0.003284931],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014082002,0.00019276516,0.4216123,0.00031162536,0.00032714652,0.0009129951,0.0018104494,0.008946395,0.08275916,0.003997804,0.184539,0.29318216],"study_design_scores_gemma":[0.0003060975,0.00013205851,0.81520844,0.00008261481,0.000070410715,0.00032665321,0.0005414443,0.016403135,0.012856075,0.002464778,0.15153189,0.00007637051],"about_ca_topic_score_codex":0.05933836,"about_ca_topic_score_gemma":0.08138137,"teacher_disagreement_score":0.05933836,"about_ca_system_score_codex":0.00075534696,"about_ca_system_score_gemma":0.0008571644,"threshold_uncertainty_score":0.117985964},"labels":[],"label_agreement":null},{"id":"W1649119254","doi":"10.1088/0004-637x/807/2/179","title":"LOCAL CIRCUMNUCLEAR MAGNETAR SOLUTION TO EXTRAGALACTIC FAST RADIO BURSTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research","funders":"","keywords":"Magnetar; Very-long-baseline interferometry; Milky Way; Galactic Center; Flux (metallurgy); Scattering; Flare","score_opus":0.019562112560083906,"score_gpt":0.2998722485592883,"score_spread":0.2803101359992044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1649119254","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6401074,0.004248702,0.24591541,0.0056155096,0.0007090909,0.00012368504,0.0016978699,0.0004454689,0.10113691],"genre_scores_gemma":[0.9612961,0.0009932481,0.016644185,0.00040419205,0.0005524374,0.00006366795,0.00073606067,0.0000967242,0.019213395],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993,0.000016211148,0.0000036885497,0.000020838228,0.000009911548,0.000019332443],"domain_scores_gemma":[0.99978465,0.00004670637,0.00005442098,0.000025832158,0.000036391888,0.000051957053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020005734,0.00031746217,0.00043194272,0.00047856287,0.00031516937,0.0008815877,0.00071089424,0.000552504,0.007033862],"category_scores_gemma":[0.0013691129,0.00016477326,0.00038759637,0.00032257487,0.00035711683,0.00048371596,0.0007615373,0.00059947727,0.0007914976],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000252756,0.00017877684,0.04660565,0.00018724587,0.00021986205,0.0027440698,0.00031186832,0.34101093,0.003973772,0.50716573,0.017565858,0.079783574],"study_design_scores_gemma":[0.00024534177,0.0002401002,0.030373495,0.00007744253,0.000108358785,0.0012527362,0.0007048328,0.6425008,0.00088415743,0.29822353,0.025325365,0.00006372254],"about_ca_topic_score_codex":0.0053781844,"about_ca_topic_score_gemma":0.0059219,"teacher_disagreement_score":0.007033862,"about_ca_system_score_codex":0.00035602532,"about_ca_system_score_gemma":0.00049808965,"threshold_uncertainty_score":0.023530602},"labels":[],"label_agreement":null},{"id":"W1649250860","doi":"10.1088/0004-637x/812/2/176","title":"ANTENNA-COUPLED TES BOLOMETERS USED IN BICEP2,<i>Keck Array</i>, AND SPIDER","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia","funders":"","keywords":"Bolometer; Detector; Cosmic microwave background; Polarimetry; Spider; Polarimeter; Interferometry; Cosmic background radiation; Microwave","score_opus":0.025975361089850626,"score_gpt":0.2557849567118016,"score_spread":0.229809595621951,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1649250860","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9548514,0.00026810382,0.036799386,0.00009937616,0.000056252524,0.00010970415,0.0006191819,0.0009483801,0.0062481947],"genre_scores_gemma":[0.93407416,0.00012784201,0.06230492,0.00012109495,0.000017339295,0.00013004274,0.0006056235,0.00011547173,0.0025034272],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99917066,0.000104532766,0.00003988254,0.0002592113,0.0003171707,0.00010856997],"domain_scores_gemma":[0.9991804,0.00008821864,0.00016154774,0.00020652813,0.00026053007,0.00010280729],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056756503,0.0003968501,0.0004548849,0.0005679633,0.00031876934,0.0007408264,0.0008719973,0.00036770102,0.0009648196],"category_scores_gemma":[0.0010359451,0.0004906027,0.00024788812,0.00077441667,0.00035588344,0.00082631275,0.0008591985,0.0004429992,0.0005935893],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005446881,0.00012200353,0.027789697,0.00017129764,0.0001324255,0.00038680053,0.0003544458,0.0051764715,0.93549794,0.0026944648,0.0011614877,0.025968317],"study_design_scores_gemma":[0.000031384883,0.00048325706,0.018641626,0.000015659036,0.00005272118,0.00046694066,0.00009765259,0.011261681,0.96147084,0.00019291764,0.0072356435,0.000049715458],"about_ca_topic_score_codex":0.0016562295,"about_ca_topic_score_gemma":0.0026793631,"teacher_disagreement_score":0.0016562295,"about_ca_system_score_codex":0.00066386757,"about_ca_system_score_gemma":0.00031003891,"threshold_uncertainty_score":0.0048166513},"labels":[],"label_agreement":null},{"id":"W1649745057","doi":"10.1086/424908","title":"Giant Pulses from PSR B1937+21 with Widths ≤15 Nanoseconds and \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $T_{b}\\geq 5\\times 10^{39}$ \\end{document} K, the Highest Brightness Temperature Observed in the Universe","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Neutron star; Atomic physics; Astrophysics; Magnetosphere; Vela; Radio telescope; Millisecond pulsar; Pulsar; Plasma; Nuclear physics","score_opus":0.01210746202026588,"score_gpt":0.2589761783405538,"score_spread":0.24686871632028792,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1649745057","genre_codex":"empirical","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.49425864,0.0010843362,0.018453984,0.0015527334,0.00083072094,0.00065343844,0.07577351,0.02687516,0.38051748],"genre_scores_gemma":[0.5385549,0.0013483074,0.015040251,0.0007002919,0.00029352444,0.00032396754,0.1497869,0.011952022,0.28199974],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9999436,0.0000034656443,0.0000032941332,0.00001093362,0.000022408907,0.0000162191],"domain_scores_gemma":[0.999783,0.000059300906,0.00002751572,0.000056418437,0.000035607813,0.00003817004],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00013741726,0.00035133376,0.00016646934,0.0006966226,0.00042882198,0.00052979426,0.0005008154,0.00043317434,0.09442525],"category_scores_gemma":[0.00047786385,0.00024083821,0.0002569949,0.0011137966,0.00015897253,0.0004617361,0.00038334788,0.00042331335,0.02203173],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001493849,0.000354623,0.018897623,0.000915031,0.00008607491,0.0013992492,0.0010806334,0.001299853,0.25305474,0.009929257,0.4464048,0.2650843],"study_design_scores_gemma":[0.00015644055,0.00025175264,0.13817485,0.00011280419,0.000054598822,0.0006078367,0.00027284052,0.0022235205,0.095135875,0.0019478917,0.76101977,0.00004189256],"about_ca_topic_score_codex":0.0028237714,"about_ca_topic_score_gemma":0.005297664,"teacher_disagreement_score":0.90557474,"about_ca_system_score_codex":0.00046551274,"about_ca_system_score_gemma":0.0002651896,"threshold_uncertainty_score":0.315884},"labels":[],"label_agreement":null},{"id":"W1650467364","doi":"10.1088/0004-637x/721/2/1056","title":"USING THE 1.6 μm BUMP TO STUDY REST-FRAME NEAR-INFRARED-SELECTED GALAXIES AT REDSHIFT 2","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Redshift; Galaxy; Stellar mass; Luminosity function; Luminosity; Photometric redshift; Redshift survey","score_opus":0.012030230443910639,"score_gpt":0.2464012554354605,"score_spread":0.23437102499154985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1650467364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9742623,0.0002608549,0.019954333,0.00006995991,0.000019972447,0.000048688744,0.001103461,0.0005766576,0.0037036985],"genre_scores_gemma":[0.9834448,0.00007530399,0.014984561,0.000028500517,0.000025575708,0.000059374972,0.00080212,0.000043850643,0.00053586497],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998305,0.00002524223,0.000005604708,0.000047086258,0.000045402838,0.000046199133],"domain_scores_gemma":[0.99833304,0.00035337344,0.00067907415,0.00030640248,0.00015079265,0.00017730122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008498135,0.00035398253,0.00033608993,0.0026032547,0.00046232122,0.00058117195,0.0005236017,0.00034732974,0.0008683719],"category_scores_gemma":[0.0018555897,0.0002408451,0.00029434165,0.001501722,0.00021479494,0.00045346402,0.0004133768,0.00033240614,0.00041762218],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003228924,0.00011714631,0.8617029,0.00009918591,0.000062421925,0.00028190383,0.00042126383,0.002592065,0.0445392,0.0033587364,0.001139208,0.08536311],"study_design_scores_gemma":[0.000018326367,0.00020400788,0.96659297,0.000021006355,0.00003942529,0.00042006618,0.00009470739,0.015201723,0.011444339,0.0016316902,0.0043125455,0.000019199788],"about_ca_topic_score_codex":0.0027113417,"about_ca_topic_score_gemma":0.004638012,"teacher_disagreement_score":0.0027113417,"about_ca_system_score_codex":0.00045481554,"about_ca_system_score_gemma":0.00015476675,"threshold_uncertainty_score":0.005391121},"labels":[],"label_agreement":null},{"id":"W1651689943","doi":"10.3847/0004-637x/821/1/64","title":"PROVIDING STRINGENT STAR FORMATION RATE LIMITS OF z ∼ 2 QSO HOST GALAXIES AT HIGH ANGULAR RESOLUTION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"QSOS; Galaxy; Star formation; Redshift; Surface brightness; Brightness; Emission spectrum; Spectrograph; Integral field spectrograph","score_opus":0.011010513154074815,"score_gpt":0.20768211096172118,"score_spread":0.19667159780764637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1651689943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99440694,0.00006994351,0.0039932844,0.000015003105,0.0000019724962,0.000005942414,0.0003385369,0.0001350188,0.0010333352],"genre_scores_gemma":[0.99615735,0.000030352638,0.003303961,0.000015127326,0.0000062847066,0.000006772485,0.0003637545,0.000009734417,0.00010663169],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998288,0.000018484989,0.000015308,0.000050720628,0.000042842614,0.000043858516],"domain_scores_gemma":[0.99907756,0.0002861134,0.00019708088,0.0001672023,0.00014974289,0.00012229633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000572169,0.00021596589,0.00026746828,0.0008677577,0.0002707253,0.00076528284,0.00026440542,0.00022904304,0.0016137218],"category_scores_gemma":[0.001436973,0.00026036685,0.00016121357,0.00032971895,0.00016903432,0.00036982878,0.00044467594,0.00015838773,0.00031757902],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030047065,0.000048064485,0.8201489,0.000040984778,0.00006432745,0.00014796956,0.00022243729,0.0034087372,0.158231,0.000593886,0.00035825136,0.016435064],"study_design_scores_gemma":[0.000021513028,0.00007649525,0.9648444,0.000009702796,0.000044842727,0.000190767,0.0001231259,0.015966076,0.017350733,0.0004013046,0.0009584534,0.00001258942],"about_ca_topic_score_codex":0.0042283637,"about_ca_topic_score_gemma":0.008282158,"teacher_disagreement_score":0.0042283637,"about_ca_system_score_codex":0.00030292833,"about_ca_system_score_gemma":0.00016417872,"threshold_uncertainty_score":0.008407474},"labels":[],"label_agreement":null},{"id":"W1651758029","doi":"10.1088/0004-637x/808/1/11","title":"ON THE DISTANCE OF THE GLOBULAR CLUSTER M4 (NGC 6121) USING RR LYRAE STARS. II. MID-INFRARED PERIOD–LUMINOSITY RELATIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"Ministero dell’Istruzione, dell’Università e della Ricerca; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"RR Lyrae variable; Globular cluster; Photometry (optics); Distance modulus; Cepheid variable; Variable star; Stars; Hubble space telescope","score_opus":0.019534723496884687,"score_gpt":0.2318935180332631,"score_spread":0.21235879453637843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1651758029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99285275,0.00048537628,0.0006408901,0.00008187313,0.000011221855,0.0000053560348,0.000843546,0.00003995855,0.0050389273],"genre_scores_gemma":[0.99702543,0.00012546472,0.0008088627,0.0000140711545,0.000017058766,0.000004986272,0.0011864292,0.000011726286,0.0008058344],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972826,0.000046423527,0.000014022977,0.00009050345,0.00008048423,0.000040262174],"domain_scores_gemma":[0.9984211,0.000414407,0.00061943807,0.00015237289,0.00019933436,0.0001933661],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053564576,0.00035539712,0.0001283476,0.002730215,0.00052020827,0.0003986628,0.00059959985,0.00046622212,0.0023154146],"category_scores_gemma":[0.002408647,0.00014373481,0.00022802851,0.0012860561,0.00037405797,0.00057852856,0.0010514465,0.00031779349,0.00079586223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022402442,0.000017309603,0.96477413,0.00006843647,0.00009894573,0.00016853643,0.00024894343,0.00485132,0.0053921347,0.0023747485,0.0019131248,0.01986836],"study_design_scores_gemma":[0.000005630591,0.000025947025,0.9935573,0.000009025598,0.000015039257,0.00009331122,0.000067832545,0.0027693948,0.00060698244,0.0004253064,0.0024173527,0.0000068230097],"about_ca_topic_score_codex":0.013971586,"about_ca_topic_score_gemma":0.019068716,"teacher_disagreement_score":0.013971586,"about_ca_system_score_codex":0.0011739273,"about_ca_system_score_gemma":0.00024646116,"threshold_uncertainty_score":0.027780533},"labels":[],"label_agreement":null},{"id":"W1652718347","doi":"10.1088/0004-637x/804/1/61","title":"SIMULTANEOUS DETECTION OF WATER, METHANE, AND CARBON MONOXIDE IN THE ATMOSPHERE OF EXOPLANET HR 8799 b","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":191,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Planet; Atmosphere (unit); Methane; Troposphere; Carbon monoxide; Abundance (ecology); Spectral line; Mixing ratio","score_opus":0.011328728941848392,"score_gpt":0.2171905323266262,"score_spread":0.2058618033847778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1652718347","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998168,0.00009639669,0.00014800666,0.000021065647,0.00000356064,0.000004445001,0.0003426959,0.000027238053,0.0011886206],"genre_scores_gemma":[0.9974566,0.000089602276,0.00047893112,0.000036281188,0.000005279675,0.000008744733,0.0014235527,0.000015000456,0.00048606604],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99988794,0.000007936674,0.0000050772624,0.000032153068,0.000038261554,0.000028586623],"domain_scores_gemma":[0.9999218,0.000007336175,0.000020578736,0.00001057514,0.000013965349,0.000025725605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011914304,0.00031321277,0.00023232593,0.00060664007,0.00047907318,0.0004511605,0.0003067755,0.00037934008,0.00075387675],"category_scores_gemma":[0.00014345562,0.00020683445,0.00019224767,0.00041160456,0.00018081936,0.00022367257,0.0005091058,0.00028390423,0.00033023866],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083118293,0.00019737233,0.42333186,0.00008515838,0.0001790598,0.001135808,0.0004764859,0.00085063826,0.5558231,0.00020039074,0.0011390079,0.015749954],"study_design_scores_gemma":[0.000018597657,0.000065345805,0.98554695,0.0000072152807,0.00002374031,0.0003260427,0.000108631204,0.0009167476,0.011677157,0.000038208495,0.0012647662,0.000006618197],"about_ca_topic_score_codex":0.0037986885,"about_ca_topic_score_gemma":0.00495083,"teacher_disagreement_score":0.0037986885,"about_ca_system_score_codex":0.00024969727,"about_ca_system_score_gemma":0.00008026538,"threshold_uncertainty_score":0.00755316},"labels":[],"label_agreement":null},{"id":"W1656361656","doi":"10.1088/0004-637x/806/1/43","title":"ON THE CLUSTER PHYSICS OF SUNYAEV–ZEL’DOVICH AND X-RAY SURVEYS. IV. CHARACTERIZING DENSITY AND PRESSURE CLUMPING DUE TO INFALLING SUBSTRUCTURES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cluster (spacecraft); RADIUS; Virial theorem; Spectral density; Galaxy cluster; Dark matter; Galaxy; Accretion (finance); Spectral line","score_opus":0.01324601487782822,"score_gpt":0.21759269260365052,"score_spread":0.2043466777258223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1656361656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98951155,0.0007720236,0.0040250984,0.00071698386,0.000020570968,0.000024861334,0.0005201098,0.000093794835,0.0043150913],"genre_scores_gemma":[0.99725574,0.0002586763,0.0015297998,0.0000823299,0.000016702073,0.000011335134,0.00035701838,0.000029922887,0.00045864983],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998233,0.00007726829,0.0000053661993,0.00003428374,0.000027948796,0.000031940817],"domain_scores_gemma":[0.99932396,0.00028404492,0.00017009108,0.000087036475,0.00005253806,0.00008232247],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009488329,0.00025449003,0.00028096003,0.00085500075,0.00040490952,0.00066400674,0.0006455428,0.00033130043,0.00096440146],"category_scores_gemma":[0.0022545133,0.00020629339,0.00034512766,0.000779336,0.0005444109,0.00064787385,0.000862706,0.0004406995,0.00010919232],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001503621,0.00007629964,0.7346741,0.00011448952,0.00035398098,0.00030993274,0.0006415898,0.19034088,0.0037962673,0.04518024,0.004453778,0.019908052],"study_design_scores_gemma":[0.000034705674,0.000047427173,0.7189011,0.00003513809,0.000029959905,0.000087025684,0.00026946655,0.26589087,0.0010159028,0.009903633,0.0037423447,0.000042496988],"about_ca_topic_score_codex":0.02258669,"about_ca_topic_score_gemma":0.020952819,"teacher_disagreement_score":0.02258669,"about_ca_system_score_codex":0.0009124859,"about_ca_system_score_gemma":0.0003453467,"threshold_uncertainty_score":0.04491049},"labels":[],"label_agreement":null},{"id":"W1657061485","doi":"10.1088/0004-637x/806/2/244","title":"THE TIME DOMAIN SPECTROSCOPIC SURVEY: VARIABLE SELECTION AND ANTICIPATED RESULTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Planetary Science Division; Leibniz-Gemeinschaft; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Max-Planck-Institut für Astrophysik; Eötvös Loránd Tudományegyetem; Queen's University Belfast; Durham University; York University; National Central University; Carnegie Institution for Science; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Max-Planck-Institut für Astronomie; University of Edinburgh; Carnegie Institution of Washington; University of Utah; Queen's University; Ohio State University; National Science Foundation; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; National Aeronautics and Space Administration","keywords":"Physics; RR Lyrae variable; Astrophysics; Quasar; Variable star; Population; Stars; Photometry (optics); Astronomy; Sky; Luminosity; Milky Way; Galaxy; Globular cluster","score_opus":0.015666550034551613,"score_gpt":0.2439165264256863,"score_spread":0.22824997639113467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1657061485","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.30438706,0.0006890984,0.6228019,0.0024580837,0.00014992176,0.0021784601,0.038972195,0.007736106,0.020627165],"genre_scores_gemma":[0.3936892,0.00044143503,0.5230529,0.0004017066,0.00015417038,0.0010043331,0.072986804,0.0006426761,0.0076268045],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.997891,0.000642708,0.00008971006,0.00023198225,0.00088623614,0.00025838087],"domain_scores_gemma":[0.99737984,0.00043360982,0.00019450761,0.0004225135,0.0013048708,0.00026457172],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0052374327,0.00040716806,0.00039855432,0.0014202503,0.0003968454,0.001186697,0.0006725345,0.0004576251,0.0030620713],"category_scores_gemma":[0.006809705,0.00025952669,0.00037994084,0.0017045619,0.00023122432,0.0006090362,0.0010240361,0.00041356497,0.0033731288],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010046154,0.00028302195,0.528448,0.0002308313,0.00013540308,0.00030477083,0.00018310489,0.032548293,0.025004497,0.01139725,0.02886058,0.3715996],"study_design_scores_gemma":[0.00034415696,0.00085749954,0.505397,0.0001092873,0.00013508326,0.0008866897,0.00055275066,0.3681809,0.03246318,0.018133437,0.07277963,0.00016038398],"about_ca_topic_score_codex":0.00781698,"about_ca_topic_score_gemma":0.0064136037,"teacher_disagreement_score":0.00781698,"about_ca_system_score_codex":0.0006841237,"about_ca_system_score_gemma":0.00089090725,"threshold_uncertainty_score":0.027698517},"labels":[],"label_agreement":null},{"id":"W1657192325","doi":"10.1086/381248","title":"High-Resolution Infrared Spectroscopy of the Brown Dwarf Indi Ba","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Brown dwarf; Surface gravity; Spectral line; Infrared; Spectral resolution; Effective temperature; Infrared spectroscopy; Spectroscopy; Astronomical spectroscopy","score_opus":0.008212627535833187,"score_gpt":0.21255064640488977,"score_spread":0.2043380188690566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1657192325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972391,0.00041034783,0.0006995109,0.000022130947,0.0000031247566,0.000001693036,0.00008512941,0.00003092503,0.0015080645],"genre_scores_gemma":[0.99703974,0.00019442421,0.001701567,0.00001560056,0.000009938076,0.000002211807,0.00034075344,0.000009383239,0.0006863268],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992085,0.000008645042,0.0000020867917,0.000022598455,0.000029455703,0.000016282675],"domain_scores_gemma":[0.9998542,0.000028067832,0.000031382868,0.000019397921,0.000039551232,0.000027374139],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001602268,0.00015656976,0.0001423588,0.0004338498,0.00028667226,0.00036349948,0.00021270596,0.00015456295,0.00032932157],"category_scores_gemma":[0.0002761034,0.00011782287,0.00011138468,0.00026985814,0.00015423537,0.00028975477,0.0002336227,0.0002525787,0.00014442118],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020288717,0.0001115866,0.18448159,0.00008056268,0.00007499334,0.0005065194,0.00034226617,0.0010082275,0.7856448,0.0005710045,0.0007341596,0.026241332],"study_design_scores_gemma":[0.000013919338,0.00010367721,0.9287737,0.000010045765,0.00005224087,0.0011833356,0.00018636626,0.00360087,0.059752174,0.00027361896,0.00603296,0.000017163287],"about_ca_topic_score_codex":0.001656522,"about_ca_topic_score_gemma":0.003070533,"teacher_disagreement_score":0.001656522,"about_ca_system_score_codex":0.0001926677,"about_ca_system_score_gemma":0.00008496274,"threshold_uncertainty_score":0.0032937527},"labels":[],"label_agreement":null},{"id":"W1661994785","doi":"10.1088/0004-637x/813/1/39","title":"SEARCHES FOR CONTINUOUS GRAVITATIONAL WAVES FROM NINE YOUNG SUPERNOVA REMNANTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Istituto Nazionale di Fisica Nucleare; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Centre National de la Recherche Scientifique; Industry Canada; Govern de les Illes Balears; Fundacja na rzecz Nauki Polskiej; European Commission; Science and Engineering Research Board; Scottish Funding Council; Institut des Origines de Lyon; Scottish Universities Physics Alliance; Hungarian Scientific Research Fund; Leverhulme Trust; Council of Scientific and Industrial Research, India; Science and Technology Facilities Council; National Research Foundation; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Supernova; Gravitational wave; Red shift; Neutron star; Galaxy","score_opus":0.03875903985513675,"score_gpt":0.3368613485096364,"score_spread":0.29810230865449966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1661994785","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991647,0.000040764546,0.0004708403,0.0000049750925,0.0000010018714,0.000005823833,0.000115637806,0.000008292395,0.0001879113],"genre_scores_gemma":[0.9975314,0.000036608548,0.0015194283,0.000008056738,0.0000033959054,0.000006618405,0.00080893596,0.0000032348967,0.00008227707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995598,0.000092362374,0.00006518304,0.00009611186,0.00012608124,0.00006042047],"domain_scores_gemma":[0.9975159,0.0008904231,0.00084375753,0.00025044798,0.00016414665,0.00033526207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008124541,0.00024984256,0.0002958984,0.0012750889,0.00044939574,0.0006424155,0.0003238416,0.00030551347,0.00036397262],"category_scores_gemma":[0.0024803458,0.0002208705,0.00030505503,0.00091804005,0.0004191699,0.00026799206,0.0008521484,0.00023605186,0.00010524164],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005896935,0.000119396645,0.94104385,0.000059863964,0.00013593327,0.0006090428,0.0005091554,0.0017914041,0.036858443,0.0005423674,0.000121215344,0.01761959],"study_design_scores_gemma":[0.000053882377,0.00043828023,0.97425395,0.000015584685,0.00013402035,0.0013558695,0.00038920194,0.003973386,0.01698109,0.0005253031,0.0018370097,0.000042417654],"about_ca_topic_score_codex":0.0017802235,"about_ca_topic_score_gemma":0.0055149803,"teacher_disagreement_score":0.0017802235,"about_ca_system_score_codex":0.00027030386,"about_ca_system_score_gemma":0.00029744388,"threshold_uncertainty_score":0.00429672},"labels":[],"label_agreement":null},{"id":"W1666235538","doi":"10.1088/0004-637x/804/2/125","title":"P-MaNGA: GRADIENTS IN RECENT STAR FORMATION HISTORIES AS DIAGNOSTICS FOR GALAXY GROWTH AND DEATH","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Star formation; Astronomy","score_opus":0.016122624590166054,"score_gpt":0.227532253430576,"score_spread":0.21140962884040995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1666235538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9875261,0.000107673295,0.001878376,0.000047841975,0.000008469451,0.000021697122,0.0076273675,0.0013243316,0.0014580685],"genre_scores_gemma":[0.9813564,0.00002840817,0.0063258507,0.00001378275,0.000011415453,0.000045925197,0.011421155,0.0003413574,0.00045565589],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996753,0.00009791745,0.000011469505,0.00011318613,0.000047701495,0.00005456339],"domain_scores_gemma":[0.9986671,0.0005706438,0.00014284522,0.00031383373,0.00007890038,0.0002265916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006677274,0.00038146353,0.0003990854,0.0011228048,0.0002719484,0.00066131103,0.0005236162,0.00020174531,0.0015546001],"category_scores_gemma":[0.001759261,0.00021187548,0.0007742071,0.0008035677,0.00032489086,0.00035039685,0.00088402035,0.00038592893,0.00044556378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014649784,0.00014003646,0.9142737,0.00015288393,0.00064030907,0.00033627043,0.000754842,0.01532589,0.013849154,0.0008240736,0.0063464283,0.04589135],"study_design_scores_gemma":[0.000034139608,0.00016843367,0.9620513,0.0000106005255,0.000053219974,0.00019374322,0.00019062277,0.03205871,0.002041444,0.00034394595,0.0028268339,0.000027058937],"about_ca_topic_score_codex":0.0057971813,"about_ca_topic_score_gemma":0.007636856,"teacher_disagreement_score":0.0057971813,"about_ca_system_score_codex":0.00024510268,"about_ca_system_score_gemma":0.00021486582,"threshold_uncertainty_score":0.011526883},"labels":[],"label_agreement":null},{"id":"W1667722556","doi":"10.1088/0004-637x/808/2/148","title":"SYSTEMATIC Non-LTE STUDY OF THE −2.6 ≤ [Fe/H] ≤ 0.2 F AND G DWARFS IN THE SOLAR NEIGHBORHOOD. I. STELLAR ATMOSPHERE PARAMETERS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Subgiant; Effective temperature; Metallicity; Surface gravity; Microturbulence; Stars; Stellar atmosphere; Spectral line; Atmospheric models; Line (geometry)","score_opus":0.014906499150683889,"score_gpt":0.22592524850935664,"score_spread":0.21101874935867274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1667722556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987752,0.00012585931,0.00030697288,0.0000055219775,0.000001636477,0.0000042065435,0.00023950159,0.000008297561,0.0005327838],"genre_scores_gemma":[0.998541,0.0000493238,0.00033840077,0.0000068877625,0.000003079693,0.0000029988478,0.00082503766,0.0000035699932,0.0002297898],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981123,0.000037950536,0.0000110265655,0.00007294154,0.000037747355,0.000029062243],"domain_scores_gemma":[0.9995347,0.000058545258,0.00009932638,0.000100095385,0.0001253525,0.00008195526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027263325,0.00012186334,0.00015976455,0.00075459224,0.0003697632,0.00018103258,0.00023242032,0.000113637296,0.00022797743],"category_scores_gemma":[0.0005490355,0.00007108106,0.0001597184,0.00047096782,0.00015507698,0.00014238691,0.0002981133,0.00007379232,0.00012471947],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006125072,0.000018658247,0.9868276,0.000013096181,0.000028970233,0.00007572635,0.0002160904,0.00017111024,0.0056940117,0.00014689405,0.00015840842,0.0065882015],"study_design_scores_gemma":[9.194629e-7,0.00001825543,0.99851245,0.0000010487026,0.0000059960576,0.00006943337,0.00006259415,0.00026605136,0.0004163947,0.000028841194,0.00061707373,9.907596e-7],"about_ca_topic_score_codex":0.011963031,"about_ca_topic_score_gemma":0.031718075,"teacher_disagreement_score":0.011963031,"about_ca_system_score_codex":0.0003015754,"about_ca_system_score_gemma":0.00021265059,"threshold_uncertainty_score":0.023786843},"labels":[],"label_agreement":null},{"id":"W1671206161","doi":"10.1086/312783","title":"[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Spectroscopy of the O [CSC]vi[/CSC] Resonance Doublet in Sand 2 (WO)","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; Université Laval; University of Victoria","funders":"","keywords":"Physics; Spectroscopy; Spectrograph; Astrophysics; Stars; Space Telescope Imaging Spectrograph; Supernova; Line (geometry); Ultraviolet; Astronomy; Resonance (particle physics); Wolf–Rayet star; Hubble space telescope; Spectral line; Atomic physics; Optics","score_opus":0.009329185360019253,"score_gpt":0.22672528110036955,"score_spread":0.2173960957403503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1671206161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9805164,0.00034107058,0.0008921722,0.00021520366,0.000075660544,0.000024471607,0.0031511474,0.0002911639,0.01449277],"genre_scores_gemma":[0.9800332,0.00026867236,0.0043105176,0.00023888673,0.00008371593,0.000019928397,0.004936618,0.00005380154,0.010054496],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997544,0.0000011055961,0.0000015426522,0.0000063094203,0.000008214334,0.000007410629],"domain_scores_gemma":[0.9999205,0.000006651621,0.000026953534,0.0000051788106,0.000010608247,0.000030128085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006809396,0.00020960072,0.000104432984,0.0010076353,0.00025394082,0.00017102095,0.00020693583,0.00021647634,0.00827204],"category_scores_gemma":[0.00007876371,0.00006957755,0.00010686015,0.0004002303,0.00010345894,0.00015975739,0.00024132778,0.00013993544,0.0009870778],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00095968944,0.00018581163,0.3341502,0.00021103624,0.000119331045,0.006258874,0.00024868708,0.00074268965,0.57194275,0.0013985934,0.02961976,0.054162674],"study_design_scores_gemma":[0.000068489106,0.00038506888,0.9122182,0.000050550334,0.00007069608,0.005709473,0.00029699202,0.002095366,0.038374327,0.0007107692,0.039995216,0.00002489683],"about_ca_topic_score_codex":0.0011362858,"about_ca_topic_score_gemma":0.0029594388,"teacher_disagreement_score":0.00827204,"about_ca_system_score_codex":0.000090947986,"about_ca_system_score_gemma":0.00006206783,"threshold_uncertainty_score":0.027672768},"labels":[],"label_agreement":null},{"id":"W1687599274","doi":"10.1088/0004-637x/695/2/1370","title":"VERITAS OBSERVATIONS OF THE BL LAC OBJECT 1ES 1218+304","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; BL Lac object; Crab Nebula; Astrophysics; Flux (metallurgy); Redshift; Spectral line; Photon; Spectral index; Light curve; MAGIC (telescope); Extragalactic background light; Astronomy; Gamma ray; Galaxy; Blazar; Optics","score_opus":0.013447766900543985,"score_gpt":0.22297934785201917,"score_spread":0.2095315809514752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1687599274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9885169,0.00046969543,0.0005985225,0.000103838094,0.000018170189,0.000018094224,0.0033191815,0.00027439636,0.006681225],"genre_scores_gemma":[0.98315585,0.00029457128,0.0032172855,0.000080009915,0.00003539738,0.000027638875,0.010487699,0.000057381098,0.0026442937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995517,0.000038688886,0.00001519205,0.00012514894,0.00018187595,0.00008750654],"domain_scores_gemma":[0.99930286,0.000070112605,0.00029844994,0.00008384084,0.000110010966,0.00013479288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005530714,0.00040967175,0.0004149369,0.0012220332,0.00046973306,0.00072653394,0.00066425547,0.00060599885,0.0025257284],"category_scores_gemma":[0.0007654053,0.00026187106,0.00026594233,0.0010210985,0.0002479408,0.0003632575,0.0006847193,0.00044054267,0.000863368],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0027441292,0.00033036905,0.46453637,0.00041412393,0.00038925983,0.0023097408,0.00092595274,0.0027771126,0.45031494,0.0032595838,0.014624416,0.057374068],"study_design_scores_gemma":[0.00012466672,0.00048853894,0.9536461,0.000039507002,0.00012252625,0.0018400538,0.0002820081,0.0031361666,0.017293809,0.0004255447,0.02254493,0.000056111803],"about_ca_topic_score_codex":0.0076130787,"about_ca_topic_score_gemma":0.018519199,"teacher_disagreement_score":0.0076130787,"about_ca_system_score_codex":0.0009935849,"about_ca_system_score_gemma":0.00033811317,"threshold_uncertainty_score":0.015137553},"labels":[],"label_agreement":null},{"id":"W1688406301","doi":"10.1088/0004-637x/813/1/46","title":"CONNECTION BETWEEN THE CIRCUMGALACTIC MEDIUM AND THE INTERSTELLAR MEDIUM OF GALAXIES: RESULTS FROM THE COS-GASS SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Science and Technology Facilities Council; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; Australian Research Council; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Galaxy; Interstellar medium; Equivalent width; RADIUS; Halo; Spectral line; Astronomy; Dark matter; Virial theorem; Impact parameter; Emission spectrum; Atomic physics","score_opus":0.022573001694089944,"score_gpt":0.23268632649748983,"score_spread":0.2101133248033999,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1688406301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99661106,0.00033185468,0.00005791698,0.000033042143,0.0000025342324,0.0000036596487,0.0024129914,0.000008169336,0.00053873117],"genre_scores_gemma":[0.9949793,0.00021171088,0.00008544876,0.000017415883,0.000012335704,0.000004257502,0.0044322177,0.0000049953005,0.00025227226],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997075,0.00006255138,0.000022579674,0.00008588389,0.000063616266,0.00005785503],"domain_scores_gemma":[0.998473,0.00022732755,0.00063049595,0.00011960143,0.00016745753,0.00038214755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042499075,0.00031627616,0.00026867155,0.0021689506,0.0002394121,0.0007649386,0.00028116824,0.0002810428,0.0015491734],"category_scores_gemma":[0.0009823977,0.00009386952,0.0002744345,0.0018965625,0.0002738177,0.00051769224,0.0008150886,0.00021445361,0.0004964834],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033315322,0.000011508352,0.99825734,0.000008806324,0.000028073986,0.000027702179,0.00006584989,0.0000423169,0.00024293452,0.00003064323,0.00013228592,0.0011192298],"study_design_scores_gemma":[0.0000017667925,0.000012190589,0.9994611,0.0000026785426,0.000011257658,0.000029981855,0.00011835976,0.0000612867,0.00003725382,0.000008211651,0.00025474298,0.0000011822844],"about_ca_topic_score_codex":0.016747035,"about_ca_topic_score_gemma":0.019145157,"teacher_disagreement_score":0.016747035,"about_ca_system_score_codex":0.00024078909,"about_ca_system_score_gemma":0.00015776882,"threshold_uncertainty_score":0.03329909},"labels":[],"label_agreement":null},{"id":"W168946373","doi":"10.1088/0004-637x/804/2/118","title":"CONSTRAINING THE RADIO-LOUD FRACTION OF QUASARS AT<i>z</i>&gt; 5.5","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Ohio Board of Regents; Max-Planck-Institut für Astronomie; Space Telescope Science Institute; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; National Central University; Durham University; Istituto Nazionale di Astrofisica; Deutsche Forschungsgemeinschaft; Universität Heidelberg; Leibniz-Gemeinschaft; University of Notre Dame; University of California, Los Angeles; Max-Planck-Gesellschaft; National Science Foundation; University of Minnesota; Queen's University; Ohio State University; Los Alamos National Laboratory; Johns Hopkins University; Queen's University Belfast; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Quasar; Physics; Astrophysics; Radio galaxy; Redshift; OVV quasar; Galaxy; Astronomy; Active galactic nucleus; COSMIC cancer database; Reionization","score_opus":0.01596587510827861,"score_gpt":0.2300306343311534,"score_spread":0.2140647592228748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W168946373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99304456,0.0004975736,0.0024103748,0.00008839895,0.000009598594,0.000010796478,0.0007028639,0.00010367055,0.003132092],"genre_scores_gemma":[0.9967891,0.00011782357,0.0014294357,0.00005518005,0.0000137070565,0.000003859666,0.0012013902,0.000010464998,0.00037914678],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981266,0.000014989073,0.000008274831,0.000053340318,0.000034961155,0.00007592388],"domain_scores_gemma":[0.99925894,0.00014168212,0.00029745363,0.000055749988,0.00007870508,0.00016745449],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055281,0.00037656285,0.00029450082,0.0015453921,0.00030388235,0.0010337515,0.00046302885,0.0004203069,0.0021254607],"category_scores_gemma":[0.0007256444,0.00020853545,0.00026909303,0.0005909027,0.0002084102,0.00032083862,0.00043171854,0.00024191987,0.0011216176],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004942108,0.000049577477,0.96962255,0.00002294356,0.00004742881,0.00007705669,0.000058956684,0.00066462153,0.012796709,0.00030334806,0.0007113264,0.0155960005],"study_design_scores_gemma":[0.0000044914045,0.000047124962,0.9925633,0.000009443392,0.000046672027,0.000111038564,0.00013338334,0.0027283917,0.0026389183,0.00011357458,0.0015974358,0.0000062000063],"about_ca_topic_score_codex":0.0056621796,"about_ca_topic_score_gemma":0.010423153,"teacher_disagreement_score":0.0056621796,"about_ca_system_score_codex":0.00017843337,"about_ca_system_score_gemma":0.00017461376,"threshold_uncertainty_score":0.011258423},"labels":[],"label_agreement":null},{"id":"W1694049600","doi":"10.1088/0004-637x/811/1/20","title":"THE POPULATION OF GALAXY–GALAXY STRONG LENSES IN FORTHCOMING OPTICAL IMAGING SURVEYS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":332,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Lens (geology); Einstein radius; Population; Redshift; RADIUS; Galaxy; Poisson distribution; Function (biology)","score_opus":0.015806279287131925,"score_gpt":0.2435381566783158,"score_spread":0.22773187739118386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1694049600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9750035,0.00048953993,0.017057681,0.0005605542,0.000017191785,0.000050859962,0.0037976282,0.00024416368,0.0027788982],"genre_scores_gemma":[0.9884952,0.00039060868,0.005466219,0.00013305827,0.00001487824,0.000039829185,0.004494245,0.00003371174,0.0009322977],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992749,0.00014932036,0.00003534295,0.00026027334,0.00014568621,0.00013443248],"domain_scores_gemma":[0.99630606,0.0013690919,0.0010124685,0.0004992916,0.00047829273,0.00033480563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018146529,0.00042216785,0.00035933903,0.00082978135,0.00042131337,0.0014570617,0.0008986977,0.000877845,0.0025680817],"category_scores_gemma":[0.009752762,0.00039903063,0.00093118916,0.0009997102,0.00074225885,0.0025331671,0.00090317783,0.00053307466,0.00063991314],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002543984,0.00007337557,0.73385805,0.00008927792,0.00015392191,0.00030645638,0.00022106867,0.23477888,0.0017992059,0.008965834,0.0032719106,0.016227541],"study_design_scores_gemma":[0.000115690564,0.00026088845,0.4676349,0.00011303603,0.0001643959,0.0008583208,0.0008015662,0.49914363,0.003428753,0.01584602,0.011508391,0.00012436051],"about_ca_topic_score_codex":0.021888694,"about_ca_topic_score_gemma":0.022446396,"teacher_disagreement_score":0.021888694,"about_ca_system_score_codex":0.0018969435,"about_ca_system_score_gemma":0.0006884496,"threshold_uncertainty_score":0.043522596},"labels":[],"label_agreement":null},{"id":"W1698916124","doi":"10.1088/0004-637x/800/2/144","title":"THE DISCOVERY OF THE FIRST “CHANGING LOOK” QUASAR: NEW INSIGHTS INTO THE PHYSICS AND PHENOMENOLOGY OF ACTIVE GALACTIC NUCLEI","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":409,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Active galactic nucleus; Quasar; Phenomenology (philosophy); Spectrograph; Telescope; Cosmology; Photon; Flux (metallurgy)","score_opus":0.01676254735999625,"score_gpt":0.22976002517684344,"score_spread":0.2129974778168472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1698916124","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99322236,0.00117273,0.0012359046,0.001125371,0.000041226038,0.000004765793,0.00014274192,0.000025651887,0.0030292477],"genre_scores_gemma":[0.99876034,0.0002901101,0.0004735427,0.00012721706,0.00004755614,0.0000016136066,0.0000807304,0.000006530397,0.00021244246],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994206,0.000008694504,0.0000028856402,0.000020265745,0.000013665387,0.000012353494],"domain_scores_gemma":[0.9994998,0.00013000176,0.00014407048,0.00007417195,0.00004312558,0.00010887764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058763765,0.000113168855,0.00016302093,0.00060024566,0.00033319203,0.0011786333,0.0003583123,0.0003736809,0.00069808133],"category_scores_gemma":[0.0013187382,0.00018213289,0.00016997577,0.00026659222,0.0012274559,0.0016170955,0.00050735165,0.00064730266,0.00007601936],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018819082,0.0001165274,0.8466174,0.00019317356,0.00011217343,0.0016852319,0.0049324525,0.00082536455,0.056355048,0.031646617,0.0026486807,0.054679137],"study_design_scores_gemma":[0.0000070782708,0.000066856934,0.97756714,0.000049379556,0.000032654953,0.0007328809,0.0014517478,0.0017564392,0.0020105646,0.010247857,0.0060487282,0.0000286462],"about_ca_topic_score_codex":0.0024631862,"about_ca_topic_score_gemma":0.004155494,"teacher_disagreement_score":0.0024631862,"about_ca_system_score_codex":0.0006577179,"about_ca_system_score_gemma":0.00016764012,"threshold_uncertainty_score":0.004897654},"labels":[],"label_agreement":null},{"id":"W1700467429","doi":"10.1088/0004-637x/809/1/98","title":"A COMBINED MAXIMUM-LIKELIHOOD ANALYSIS OF THE HIGH-ENERGY ASTROPHYSICAL NEUTRINO FLUX MEASURED WITH ICECUBE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":480,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; U.S. Department of Energy; University of Wisconsin-Madison; Vetenskapsrådet; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; Vlaamse regering; University of Oxford; Compute Canada; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Neutrino; Flux (metallurgy); Astrophysics; Muon; Spectral index; Zenith; Power law; Astroparticle physics; Particle physics; Nuclear physics; Astronomy; Spectral line; Statistics","score_opus":0.00973259751961893,"score_gpt":0.20173845080832814,"score_spread":0.1920058532887092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1700467429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8734206,0.00068301405,0.112427965,0.00023088169,0.000012188239,0.00007406305,0.00630879,0.0007525647,0.0060899607],"genre_scores_gemma":[0.92373645,0.00028766604,0.060026124,0.000055742246,0.000031056017,0.000116295996,0.014186829,0.0002456997,0.0013141854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99879265,0.0006299795,0.000050793704,0.00021258938,0.00023664052,0.000077366996],"domain_scores_gemma":[0.9979571,0.0013618481,0.00023039186,0.00023193967,0.00015921351,0.000059505317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032198739,0.0010610915,0.0010419218,0.0018972091,0.0004351456,0.0019141828,0.0007852891,0.00039900478,0.001471657],"category_scores_gemma":[0.0053577865,0.00058213633,0.001708814,0.0020085883,0.000420247,0.00095319614,0.0010907203,0.0006300275,0.00047523648],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0032969192,0.0003051531,0.4340997,0.00029511566,0.0029799144,0.000588223,0.00037328785,0.42023468,0.026992548,0.009604228,0.0030575453,0.0981727],"study_design_scores_gemma":[0.00013872352,0.0001945513,0.24444273,0.00005381499,0.00033590727,0.0005507592,0.00020757235,0.719549,0.019109586,0.010209448,0.0050820373,0.00012592974],"about_ca_topic_score_codex":0.005234167,"about_ca_topic_score_gemma":0.0051243487,"teacher_disagreement_score":0.005234167,"about_ca_system_score_codex":0.00083229796,"about_ca_system_score_gemma":0.00069771655,"threshold_uncertainty_score":0.01702851},"labels":[],"label_agreement":null},{"id":"W1700605073","doi":"10.1088/0004-637x/806/2/255","title":"ON ORIGIN AND DESTRUCTION OF RELATIVISTIC DUST AND ITS IMPLICATION FOR ULTRAHIGH ENERGY COSMIC RAYS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic ray; Astrophysics; Relativistic particle; Radiation; Cosmic dust; Lorentz factor; Interstellar medium; Photoelectric effect; Atomic physics; Galaxy; Nuclear physics; Lorentz transformation; Electron","score_opus":0.0166960281012761,"score_gpt":0.2424722905324097,"score_spread":0.2257762624311336,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1700605073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.976458,0.0075871414,0.009346475,0.00022758299,0.000033635017,0.000014849916,0.000084258965,0.00006474545,0.0061832624],"genre_scores_gemma":[0.99574727,0.0016314965,0.0018146489,0.00001690475,0.000013165483,0.000004032291,0.00004065671,0.000012466433,0.0007193575],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998863,0.000014903196,0.000005485179,0.000035484536,0.00002620741,0.000031675303],"domain_scores_gemma":[0.9997929,0.00006017713,0.00007698872,0.000027220798,0.000022335724,0.00002041923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024105668,0.00032709684,0.0002784809,0.0005746895,0.00044344203,0.0010038667,0.00068978505,0.0005797183,0.0007213445],"category_scores_gemma":[0.00043061867,0.00023024621,0.0004947471,0.00040236994,0.00067278935,0.0008046512,0.00039066494,0.00029617953,0.000183694],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011051969,0.0003095035,0.44446245,0.0011309038,0.00026376414,0.005274876,0.0010475771,0.108151466,0.2019736,0.13516347,0.0013925831,0.099724606],"study_design_scores_gemma":[0.00007365925,0.00079339324,0.61012703,0.00014872568,0.00021685653,0.003337874,0.0017751423,0.20133586,0.11590816,0.05318002,0.012977586,0.000125739],"about_ca_topic_score_codex":0.0027003414,"about_ca_topic_score_gemma":0.0016677101,"teacher_disagreement_score":0.0027003414,"about_ca_system_score_codex":0.00082160934,"about_ca_system_score_gemma":0.00016118068,"threshold_uncertainty_score":0.0059611797},"labels":[],"label_agreement":null},{"id":"W1701063863","doi":"10.1088/0004-637x/806/1/111","title":"THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: RAPID C iv BROAD ABSORPTION LINE VARIABILITY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; University of Cambridge; Natural Sciences and Engineering Research Council of Canada; York University; Space Telescope Science Institute; Carnegie Mellon University; University of Arizona; Office of Science; Princeton University; University of Washington; Alfred P. Sloan Foundation; College of Engineering, Michigan State University; Johns Hopkins University; University of Michigan; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; George Mason University; American Academy of Periodontology Foundation; National Science Foundation; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Quasar; Reverberation mapping; Astrophysics; Physics; Sky; Emission spectrum; Galaxy; Astronomy; Outflow; Absorption spectroscopy; RADIUS; Spectral line; Meteorology; Optics","score_opus":0.022880102964675263,"score_gpt":0.23809135439221865,"score_spread":0.21521125142754338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1701063863","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98800385,0.0003087298,0.0014169036,0.00019023249,0.000029862467,0.00003084939,0.006941537,0.00024191359,0.0028361052],"genre_scores_gemma":[0.97621876,0.00025754666,0.0032520718,0.000094084135,0.000044738466,0.000029846728,0.019204209,0.00008392864,0.00081489916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962485,0.00004564332,0.000015703574,0.0000864027,0.00013802122,0.00008941123],"domain_scores_gemma":[0.99888295,0.00008706048,0.0004350648,0.00017589098,0.00016792408,0.00025104632],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089120405,0.0002687525,0.00018178293,0.0013059997,0.00032445783,0.0007580164,0.00029499058,0.00021999596,0.00056515983],"category_scores_gemma":[0.00077461737,0.00012539752,0.00018710947,0.0012871718,0.00019533078,0.00027860756,0.0007201017,0.00028167962,0.0002937095],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018971693,0.00015678769,0.9184311,0.00008508334,0.00013955004,0.00081912155,0.0007329328,0.00083622057,0.020880992,0.00045172,0.011026633,0.04625018],"study_design_scores_gemma":[0.0000058727096,0.00001725924,0.9951047,0.0000045741635,0.0000093966355,0.00015068047,0.000059844024,0.00047487003,0.00058301404,0.000055791348,0.0035282224,0.0000060194925],"about_ca_topic_score_codex":0.010393757,"about_ca_topic_score_gemma":0.024104128,"teacher_disagreement_score":0.010393757,"about_ca_system_score_codex":0.00031619205,"about_ca_system_score_gemma":0.00037548406,"threshold_uncertainty_score":0.02066654},"labels":[],"label_agreement":null},{"id":"W1744848446","doi":"10.1088/0004-637x/805/1/2","title":"TiNy TITANS: THE ROLE OF DWARF–DWARF INTERACTIONS IN LOW-MASS GALAXY EVOLUTION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University","funders":"","keywords":"Dwarf galaxy; Galaxy; Dwarf spheroidal galaxy; Star formation; Irregular galaxy; Interstellar medium; Local Group; Interacting galaxy","score_opus":0.01499015599401741,"score_gpt":0.28133710075713647,"score_spread":0.26634694476311904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1744848446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99154633,0.0006405283,0.0050389143,0.000094108065,0.000012574347,0.000019964416,0.0007146918,0.00011926648,0.0018136735],"genre_scores_gemma":[0.9923218,0.00021572383,0.00610377,0.00003628386,0.000025092379,0.000016358112,0.000793436,0.00003114722,0.0004563343],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998838,0.000016615024,0.0000061981095,0.000046084184,0.000029317345,0.000018036091],"domain_scores_gemma":[0.9994911,0.00010202816,0.00018937326,0.000063776635,0.000030859133,0.00012293526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003202955,0.0001544828,0.00019036194,0.00061801384,0.0003257596,0.00074265397,0.00032643112,0.00013934293,0.00055287953],"category_scores_gemma":[0.0009577935,0.00012939778,0.00016898305,0.0006702547,0.00040337924,0.0004968759,0.00075388857,0.00022516008,0.000101505764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014948295,0.000031174914,0.9116239,0.00009507344,0.00008215547,0.00041883113,0.00077059487,0.0019507813,0.037425775,0.0043534166,0.00090637256,0.04219245],"study_design_scores_gemma":[0.000004533239,0.00006409427,0.97886014,0.000012883416,0.000026103564,0.0005540439,0.0001882131,0.0061519695,0.0038263404,0.002830377,0.0074657532,0.000015548016],"about_ca_topic_score_codex":0.0050080763,"about_ca_topic_score_gemma":0.008280736,"teacher_disagreement_score":0.0050080763,"about_ca_system_score_codex":0.00029877486,"about_ca_system_score_gemma":0.000246401,"threshold_uncertainty_score":0.00995785},"labels":[],"label_agreement":null},{"id":"W1747229830","doi":"10.1088/0004-637x/810/1/50","title":"A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND GRAVITATIONAL LENSING POTENTIAL FROM 100 SQUARE DEGREES OF SPTPOL DATA","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Three-Speed Logic (Canada); Canadian Institute for Advanced Research; McGill University","funders":"Argonne National Laboratory; Compute Canada; Office of Science; University of Chicago; U.S. Department of Energy","keywords":"Cosmic microwave background; Gravitational lens; South Pole Telescope; Polarization (electrochemistry); Weak gravitational lensing; Sky; Cosmology; Telescope; Cosmic background radiation","score_opus":0.0569306211985414,"score_gpt":0.27833512498208063,"score_spread":0.22140450378353924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1747229830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9871242,0.00007322417,0.0042722337,0.000062074585,0.000005276058,0.000019072868,0.00535603,0.00018346687,0.0029044459],"genre_scores_gemma":[0.9818604,0.00009149691,0.0060423,0.000023265753,0.000025682524,0.00003982874,0.011505616,0.000073478346,0.00033794748],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99924624,0.00015650295,0.000026727734,0.00015218921,0.00032144156,0.0000970456],"domain_scores_gemma":[0.99787164,0.0007011665,0.0005639116,0.00033681307,0.0003053664,0.00022099384],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056029164,0.00049280224,0.00029555897,0.0023087051,0.00033682014,0.00064885855,0.00038979237,0.00024683695,0.001128302],"category_scores_gemma":[0.0030623595,0.0002823031,0.0003740145,0.002828512,0.00024431478,0.00046356808,0.0006822596,0.00052053586,0.00051189034],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042295599,0.0001241654,0.906081,0.00010761495,0.00037231346,0.0004041918,0.00029981005,0.017268347,0.02703321,0.0010872519,0.0023801865,0.04441889],"study_design_scores_gemma":[0.000023687684,0.00009256926,0.9756056,0.000010870112,0.00004301263,0.0002262254,0.000088892935,0.01445278,0.0066693267,0.0003825902,0.0023775385,0.000026930378],"about_ca_topic_score_codex":0.0049711717,"about_ca_topic_score_gemma":0.009715204,"teacher_disagreement_score":0.0049711717,"about_ca_system_score_codex":0.00037793414,"about_ca_system_score_gemma":0.00024180088,"threshold_uncertainty_score":0.009884477},"labels":[],"label_agreement":null},{"id":"W1755419543","doi":"10.1088/0004-637x/811/1/43","title":"AN ULTRASOFT X-RAY FLARE FROM 3XMM J152130.7+074916: A TIDAL DISRUPTION EVENT CANDIDATE","year":2015,"lang":"es","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Flare; Supermassive black hole; Accretion (finance); Outflow; RADIUS; Galaxy; Luminosity; Galactic Center","score_opus":0.015447132485157762,"score_gpt":0.2644168049495495,"score_spread":0.24896967246439175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1755419543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974711,0.00032931656,0.00026532414,0.00013063654,0.000028351487,0.000014097852,0.0003454789,0.000051747316,0.0013640261],"genre_scores_gemma":[0.99679273,0.00012736216,0.000714849,0.00011740293,0.00006773759,0.000013732031,0.0011917484,0.000018081306,0.0009563465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998896,0.000005535403,0.0000078650155,0.000035169214,0.00002582748,0.000035951452],"domain_scores_gemma":[0.9996012,0.000021536132,0.00015034838,0.000038599843,0.000029966672,0.00015839328],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018132212,0.00038868978,0.00045477867,0.0006621134,0.0006238742,0.00071434316,0.000648132,0.0008449237,0.0017782263],"category_scores_gemma":[0.00032512605,0.00020205873,0.00039402215,0.0006160291,0.0003317002,0.00034654752,0.00094216474,0.00038890605,0.0006571744],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006950213,0.0003086851,0.7834165,0.00017411278,0.00019656804,0.031513106,0.0008765522,0.0008205401,0.14983496,0.0015435847,0.003269541,0.027350832],"study_design_scores_gemma":[0.00006564463,0.0005078705,0.955532,0.000047568705,0.000095795156,0.015960721,0.00036573832,0.003180579,0.009958024,0.0007702516,0.013461609,0.000054198073],"about_ca_topic_score_codex":0.0015624207,"about_ca_topic_score_gemma":0.0027597162,"teacher_disagreement_score":0.0017782263,"about_ca_system_score_codex":0.00038919997,"about_ca_system_score_gemma":0.00020200381,"threshold_uncertainty_score":0.0059487224},"labels":[],"label_agreement":null},{"id":"W1755448092","doi":"10.1086/379345","title":"Improved Measurement of the Angular Power Spectrum of Temperature Anisotropy in the Cosmic Microwave Background from Two New Analyses of BOOMERANG Observations","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Astrophysics; Spectral density; Cold dark matter; Spectral index; Anisotropy; Cosmic background radiation; Dark energy; Spectral line; Universe; Cosmology; COSMIC cancer database; Dark matter; Astronomy; Optics","score_opus":0.02984592116277841,"score_gpt":0.2762002219240344,"score_spread":0.24635430076125597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1755448092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9920711,0.00023176149,0.0043861857,0.000045593824,0.000009959362,0.000018164115,0.0009148812,0.000107370484,0.0022149207],"genre_scores_gemma":[0.9855666,0.00018168532,0.009847275,0.000034873898,0.00003242477,0.00003185988,0.0033828435,0.00006199893,0.000860426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996505,0.000053426756,0.000015660158,0.00009587852,0.0000956522,0.0000888697],"domain_scores_gemma":[0.9992428,0.00010334879,0.00020681697,0.00013909025,0.0002007393,0.00010729135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046410842,0.00067668036,0.00028795944,0.0022031225,0.0003965565,0.00060310523,0.00025712556,0.00019436449,0.00069691014],"category_scores_gemma":[0.00088843616,0.00028657334,0.00033684136,0.0012000867,0.0002644972,0.0003527857,0.0007207411,0.00041735836,0.00022893018],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094716734,0.00020350028,0.6720393,0.0001280057,0.00038750714,0.0005688087,0.0016161413,0.001396322,0.23014896,0.0008160803,0.0013717406,0.090376504],"study_design_scores_gemma":[0.000013838766,0.00003664732,0.9860066,0.0000058237356,0.000053502106,0.0002853654,0.000045900633,0.0010103066,0.009446071,0.00008767833,0.0029859485,0.00002227583],"about_ca_topic_score_codex":0.0077076405,"about_ca_topic_score_gemma":0.033253524,"teacher_disagreement_score":0.0077076405,"about_ca_system_score_codex":0.00042544838,"about_ca_system_score_gemma":0.00015584023,"threshold_uncertainty_score":0.015325606},"labels":[],"label_agreement":null},{"id":"W1769353942","doi":"10.1088/0004-637x/727/2/83","title":"A PANCHROMATIC STUDY OF BLAST COUNTERPARTS: TOTAL STAR FORMATION RATE, MORPHOLOGY, ACTIVE GALACTIC NUCLEUS FRACTION, AND STELLAR MASS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia","funders":"Office of Polar Programs; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Canadian Space Agency; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Stellar mass; Spiral galaxy; Astronomy; Active galactic nucleus; Stellar population","score_opus":0.010287458884165638,"score_gpt":0.21094636908956343,"score_spread":0.2006589102053978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1769353942","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99893445,0.000017270284,0.0002768347,0.0000049797886,4.505354e-7,0.0000040835434,0.00049661874,0.000016214959,0.00024917556],"genre_scores_gemma":[0.997654,0.000019494544,0.000762478,0.0000054387433,0.000002978035,0.000005161256,0.001333456,0.000011723255,0.00020528512],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984396,0.000020744812,0.00001174014,0.000060177164,0.000029749883,0.000033633383],"domain_scores_gemma":[0.99873275,0.00024868068,0.0005042072,0.00016046005,0.00011815423,0.00023585693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030257186,0.00035500483,0.00032348675,0.0015541621,0.00024729135,0.0004590028,0.000272873,0.00023822917,0.0013171842],"category_scores_gemma":[0.0011866026,0.00021905972,0.00043220466,0.0012141591,0.00018178727,0.00041037626,0.00049536425,0.00022776386,0.00055922515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060386457,0.000020170162,0.99356717,0.000004834652,0.00004284557,0.00005791231,0.000053415013,0.00066023116,0.0033131663,0.000035243,0.000053491935,0.0021311943],"study_design_scores_gemma":[0.000001946727,0.00003199377,0.9971789,8.573874e-7,0.000009087372,0.00012990947,0.000039139893,0.0021538986,0.00035711416,0.000017215636,0.00007810303,0.0000018436199],"about_ca_topic_score_codex":0.0037452623,"about_ca_topic_score_gemma":0.0059271543,"teacher_disagreement_score":0.0037452623,"about_ca_system_score_codex":0.00019946079,"about_ca_system_score_gemma":0.00010839373,"threshold_uncertainty_score":0.0074469447},"labels":[],"label_agreement":null},{"id":"W1771452208","doi":"10.1088/0004-637x/779/1/67","title":"SPT 0538–50: PHYSICAL CONDITIONS IN THE INTERSTELLAR MEDIUM OF A STRONGLY LENSED DUSTY STAR-FORMING GALAXY AT<i>z</i>= 2.8","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Star formation; Interstellar medium; Redshift; Millimeter; Luminosity","score_opus":0.00891480699035477,"score_gpt":0.21933156287685113,"score_spread":0.21041675588649636,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1771452208","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99868125,0.00003421448,0.00005823522,0.000012046456,0.0000013243766,0.0000042757356,0.00033725228,0.000015409252,0.0008560052],"genre_scores_gemma":[0.99890995,0.00003318374,0.0002678529,0.000008618809,0.000007150766,0.0000033617591,0.0006829982,0.000003938031,0.00008296343],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987996,0.00000741528,0.000005862507,0.000042014344,0.000031137843,0.000033619588],"domain_scores_gemma":[0.99972874,0.000021406328,0.000117900316,0.000022265875,0.000013595405,0.000096069256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012849958,0.0003664421,0.00026694068,0.0009765695,0.0005476003,0.00063811225,0.00045015506,0.00033114568,0.0011539238],"category_scores_gemma":[0.0003371647,0.0002148269,0.00016470824,0.00083602144,0.00045818882,0.0005527086,0.0008061992,0.00029304493,0.0003413813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028316787,0.00016708767,0.94957614,0.000054977052,0.00008876845,0.0023692674,0.0009940851,0.0012227718,0.034787863,0.00062830513,0.001015323,0.008812169],"study_design_scores_gemma":[0.0000147175415,0.000070464135,0.9953703,0.000005481332,0.000013937531,0.0007629806,0.00021205198,0.0014156435,0.0010997215,0.00014616195,0.0008804415,0.000008063532],"about_ca_topic_score_codex":0.005915139,"about_ca_topic_score_gemma":0.009587675,"teacher_disagreement_score":0.005915139,"about_ca_system_score_codex":0.00044711764,"about_ca_system_score_gemma":0.0001426689,"threshold_uncertainty_score":0.011761427},"labels":[],"label_agreement":null},{"id":"W1771508005","doi":"10.3847/0004-637x/821/1/39","title":"RADIAL TRENDS IN IMF-SENSITIVE ABSORPTION FEATURES IN TWO EARLY-TYPE GALAXIES: EVIDENCE FOR ABUNDANCE-DRIVEN GRADIENTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Velocity dispersion; Radial velocity; Absorption (acoustics); Metallicity; Galaxy; Dispersion (optics); Spectral line; Absorption spectroscopy","score_opus":0.01639116462615138,"score_gpt":0.27367241843360357,"score_spread":0.2572812538074522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1771508005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985877,0.00005484953,0.00032742048,0.000022082544,0.0000011604527,0.0000030691733,0.00026792716,0.000074965625,0.00066074403],"genre_scores_gemma":[0.9989956,0.000012954268,0.00040185693,0.0000181551,0.00000244344,0.0000036312415,0.00027355918,0.00001159835,0.00028019122],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998865,0.000011953207,0.000007527794,0.000035198937,0.000023073988,0.000035714114],"domain_scores_gemma":[0.9986935,0.00019591431,0.00036249784,0.00011919874,0.00031195168,0.00031697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003030985,0.00021480968,0.00023404589,0.0014125368,0.00021850753,0.0004266794,0.00034899233,0.00040911834,0.0014287368],"category_scores_gemma":[0.000691913,0.0002988139,0.0001723236,0.0005599334,0.00025371066,0.00024829473,0.00035953606,0.00032650362,0.0005350378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044145738,0.0001611228,0.8219898,0.000026622343,0.00006671559,0.00020622036,0.00032861167,0.0004243988,0.16906808,0.00013369083,0.0003894445,0.006763892],"study_design_scores_gemma":[0.0000038508097,0.000027811238,0.9953826,0.0000016868925,0.000006894296,0.00008137644,0.00002939955,0.0004095095,0.0039033543,0.000020710217,0.0001279855,0.0000047451135],"about_ca_topic_score_codex":0.0043334067,"about_ca_topic_score_gemma":0.005199759,"teacher_disagreement_score":0.0043334067,"about_ca_system_score_codex":0.0003592032,"about_ca_system_score_gemma":0.00008352463,"threshold_uncertainty_score":0.008616388},"labels":[],"label_agreement":null},{"id":"W1772677041","doi":"10.1088/0004-637x/805/1/35","title":"X-RAY CAVITIES IN A SAMPLE OF 83 SPT-SELECTED CLUSTERS OF GALAXIES: TRACING THE EVOLUTION OF AGN FEEDBACK IN CLUSTERS OF GALAXIES OUT TO<i>z</i>= 1.2","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Supermassive black hole; Intracluster medium; Active galactic nucleus; Galaxy cluster; Galaxy; Redshift; Astronomy; Accretion (finance); Surface brightness; Cluster (spacecraft)","score_opus":0.0124439702529168,"score_gpt":0.22365626734147057,"score_spread":0.21121229708855377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1772677041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99972945,0.000016785696,0.000024373436,0.0000030124727,2.1765206e-7,0.0000032417029,0.00015848281,0.0000033555898,0.000061123006],"genre_scores_gemma":[0.99906677,0.00003709362,0.00011953544,0.0000066072726,0.0000026576656,0.000007838978,0.000608615,0.0000037312473,0.00014716829],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976546,0.000026401456,0.000015080544,0.00007861029,0.000040813065,0.000073589734],"domain_scores_gemma":[0.9986582,0.00014143014,0.00046964287,0.00013915225,0.00015171446,0.00043992169],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034141954,0.0002997818,0.00028109775,0.0012141532,0.0004930637,0.0005442737,0.00041065004,0.00033048054,0.00087969087],"category_scores_gemma":[0.0007588233,0.00032111554,0.00029341312,0.000969709,0.0003720213,0.00035475055,0.00090903393,0.00031945383,0.00051244715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000038714414,0.00002230698,0.99741936,0.0000034486436,0.000015817428,0.00007065439,0.0002831034,0.000037712216,0.0010655603,0.000012327005,0.00005718069,0.00097385223],"study_design_scores_gemma":[0.000001103307,0.000022122691,0.9995889,5.377755e-7,0.0000033908912,0.00008063688,0.00012595019,0.00006665506,0.000068076566,0.000002680196,0.00003915719,7.535561e-7],"about_ca_topic_score_codex":0.012135113,"about_ca_topic_score_gemma":0.015564187,"teacher_disagreement_score":0.012135113,"about_ca_system_score_codex":0.00029227763,"about_ca_system_score_gemma":0.00018810657,"threshold_uncertainty_score":0.024128973},"labels":[],"label_agreement":null},{"id":"W1775749252","doi":"10.1088/0004-637x/811/1/40","title":"FARADAY TOMOGRAPHY OF THE NORTH POLAR SPUR: CONSTRAINTS ON THE DISTANCE TO THE SPUR AND ON THE MAGNETIC FIELD OF THE GALAXY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan College; Canadian Institute for Theoretical Astrophysics; National Research Council Canada; Dominion Astrophysical Observatory; University of Toronto; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Faraday effect; Physics; Faraday cage; Galaxy; Polarization (electrochemistry); Astrophysics; Milky Way; Magnetic field; Interstellar medium; Astronomy; Chemistry","score_opus":0.008099992240831891,"score_gpt":0.1999595683521953,"score_spread":0.19185957611136342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1775749252","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86673033,0.005743841,0.007823059,0.004387715,0.0003208271,0.000021360209,0.0018674831,0.00033903032,0.11276636],"genre_scores_gemma":[0.9969348,0.0006686611,0.00076784345,0.00007976351,0.00015586852,0.000003178344,0.00039448257,0.000026211965,0.00096915255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988234,0.000021743203,0.000002803546,0.000027009164,0.000040872837,0.000025092066],"domain_scores_gemma":[0.99932504,0.00014119671,0.00016512984,0.00006920114,0.00015238479,0.00014716564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040058244,0.00027012583,0.00036640174,0.00079721335,0.0004651091,0.00089985615,0.00024034617,0.0003335057,0.0027858699],"category_scores_gemma":[0.0017214549,0.00020964148,0.00014968446,0.00081115257,0.0005113444,0.00066467025,0.0010066009,0.0005989287,0.0005445176],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013576552,0.00009310409,0.6691293,0.00061905314,0.00033356991,0.0015297066,0.0024375832,0.016582387,0.07603669,0.043947592,0.035552796,0.15238057],"study_design_scores_gemma":[0.000117173055,0.000052139127,0.96000123,0.00009846092,0.0000750477,0.00034076368,0.00062733324,0.007822999,0.0026564365,0.008053121,0.020109115,0.000046064783],"about_ca_topic_score_codex":0.006860177,"about_ca_topic_score_gemma":0.01103294,"teacher_disagreement_score":0.006860177,"about_ca_system_score_codex":0.0004159515,"about_ca_system_score_gemma":0.00040320854,"threshold_uncertainty_score":0.013640463},"labels":[],"label_agreement":null},{"id":"W1776530701","doi":"10.1086/515395","title":"The Extended Star Formation History of the Andromeda Spheroid at 21 kpc on the Minor Axis","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Metallicity; Physics; Population; Star formation; Astronomy; Galaxy; Andromeda; Stellar population; Advanced Camera for Surveys; Demography; Milky Way","score_opus":0.008829143526854832,"score_gpt":0.19685491992988496,"score_spread":0.18802577640303014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1776530701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94759023,0.0014221789,0.00044346479,0.0004384841,0.000065769986,0.000028326594,0.016621124,0.00020172403,0.033188783],"genre_scores_gemma":[0.9884243,0.00030365688,0.00044409215,0.000030892817,0.000021691354,0.0000069204357,0.007493105,0.000025820435,0.0032494892],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999163,0.00001004421,0.000003819499,0.000029495683,0.000016061289,0.000024277208],"domain_scores_gemma":[0.9994617,0.00004730893,0.00010897333,0.000034449968,0.00015797114,0.0001895858],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012664932,0.00026803117,0.00020275466,0.0011647724,0.00052463636,0.0007199308,0.00023315896,0.00022644928,0.0070734],"category_scores_gemma":[0.0005199284,0.00013935541,0.00029716836,0.0007485347,0.00017120515,0.00033174513,0.0005961305,0.0003959698,0.0010741282],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054789387,0.00007956667,0.90591735,0.00020743336,0.0003210919,0.0005025767,0.0011707172,0.010110006,0.020386098,0.0036922242,0.01670412,0.04036083],"study_design_scores_gemma":[0.0000056254494,0.000022171136,0.99284595,0.000011997078,0.000014229937,0.00006433726,0.00013737881,0.0007568726,0.00017749626,0.00010205222,0.005853234,0.000008708945],"about_ca_topic_score_codex":0.03409131,"about_ca_topic_score_gemma":0.04284202,"teacher_disagreement_score":0.03409131,"about_ca_system_score_codex":0.0006517311,"about_ca_system_score_gemma":0.00034222333,"threshold_uncertainty_score":0.06778574},"labels":[],"label_agreement":null},{"id":"W1778512384","doi":"10.1088/0004-637x/807/1/46","title":"SEARCHES FOR TIME-DEPENDENT NEUTRINO SOURCES WITH ICECUBE DATA FROM 2008 TO 2012","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Office of Polar Programs; Bundesministerium für Bildung und Forschung; Marsden Fund; Japan Society for the Promotion of Science; U.S. Department of Energy; Vetenskapsrådet; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Vlaamse regering; University of Oxford; Compute Canada; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Neutrino; Neutrino astronomy; Supernova; Neutrino detector; Measurements of neutrino speed; Solar neutrino problem; Neutrino oscillation","score_opus":0.04025071336373945,"score_gpt":0.26314179908408725,"score_spread":0.2228910857203478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1778512384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9511411,0.0010333038,0.003948671,0.00015375961,0.000054210297,0.00008525793,0.033940185,0.00030103177,0.009342617],"genre_scores_gemma":[0.8561873,0.0011772405,0.015029827,0.0001005525,0.00012813836,0.00023185916,0.12341758,0.00015468958,0.00357284],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996482,0.000045720717,0.000026241081,0.000093814786,0.00012873542,0.00005734592],"domain_scores_gemma":[0.99887615,0.00026350628,0.00046327972,0.00013042157,0.00019184078,0.00007470975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007896759,0.00028003473,0.00042367732,0.0023868051,0.00037891034,0.00092273863,0.00033840275,0.00030538853,0.0017945648],"category_scores_gemma":[0.001752104,0.00019808766,0.0004249786,0.0028690365,0.00018471359,0.0004946388,0.0005835963,0.00029585583,0.0003992483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020394872,0.00017568146,0.8539762,0.00042895362,0.0006881895,0.0014050301,0.0008590731,0.010787247,0.02512615,0.002417034,0.011816679,0.09028032],"study_design_scores_gemma":[0.00005974065,0.00018158487,0.92659897,0.00010346641,0.00024728113,0.0007648721,0.0003137712,0.0055781947,0.01396984,0.0007717045,0.05135885,0.000051607232],"about_ca_topic_score_codex":0.0067060958,"about_ca_topic_score_gemma":0.015962642,"teacher_disagreement_score":0.0067060958,"about_ca_system_score_codex":0.00061785954,"about_ca_system_score_gemma":0.0006673361,"threshold_uncertainty_score":0.0133340955},"labels":[],"label_agreement":null},{"id":"W1782044501","doi":"10.1088/0004-637x/728/2/98","title":"THE RADIATIVE EFFICIENCY OF ACCRETION FLOWS IN INDIVIDUAL ACTIVE GALACTIC NUCLEI","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":327,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Radiative transfer; Accretion (finance); Luminosity; Quasar; Astronomy; Black hole (networking); Velocity dispersion; Galaxy","score_opus":0.013752113786185382,"score_gpt":0.22122156013946984,"score_spread":0.20746944635328446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1782044501","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99081504,0.000668655,0.0037487797,0.000024354338,0.000005962217,0.00000980975,0.00029408684,0.000067684494,0.0043657143],"genre_scores_gemma":[0.9979862,0.00027072505,0.00080626184,0.000014073878,0.000011343481,0.000010776851,0.000343986,0.000017376433,0.0005393086],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997265,0.00004956452,0.000022754943,0.00010248464,0.000054485634,0.000044234745],"domain_scores_gemma":[0.99904495,0.00041655576,0.00025957273,0.00013505969,0.00010061451,0.00004311788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072080747,0.0003439514,0.00022661644,0.0012333468,0.00027293546,0.0010695597,0.000582186,0.0002106823,0.0009367522],"category_scores_gemma":[0.002530854,0.0002430861,0.00029276233,0.00060549803,0.0003871036,0.0006923985,0.0006456191,0.00020959073,0.0005315076],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016201525,0.00005431351,0.8331533,0.00011844475,0.0002138222,0.00021142465,0.00041415507,0.010972777,0.1144195,0.0030682308,0.00027078684,0.03694131],"study_design_scores_gemma":[0.000011623744,0.000067139015,0.93997633,0.000020364694,0.00006318831,0.0005704868,0.00015727532,0.023568643,0.031385187,0.0023218973,0.0018277145,0.00003008467],"about_ca_topic_score_codex":0.0019174389,"about_ca_topic_score_gemma":0.0013528558,"teacher_disagreement_score":0.0019174389,"about_ca_system_score_codex":0.00064123084,"about_ca_system_score_gemma":0.00014549377,"threshold_uncertainty_score":0.0046524405},"labels":[],"label_agreement":null},{"id":"W1783912015","doi":"10.1088/0004-637x/807/1/48","title":"A MULTIWAVELENGTH STUDY OF THREE HYBRID BLAZARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Smithsonian Astrophysical Observatory; Associated Universities; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Space Telescope Science Institute; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Blazar; Cosmic microwave background; Active galactic nucleus; Radio galaxy; Synchrotron; Quasar; Population; Astronomy; Galaxy; Gamma ray; Optics; Anisotropy","score_opus":0.022369700216059454,"score_gpt":0.24166325542958958,"score_spread":0.2192935552135301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1783912015","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986796,0.000053474218,0.00025386424,0.000009050173,0.0000011082947,0.0000036852616,0.000052948086,0.000015002057,0.0009313888],"genre_scores_gemma":[0.9991357,0.00001981074,0.00050536636,0.000007783215,0.000002740903,0.000002216687,0.00012679037,0.0000056736476,0.00019388317],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998971,0.000010360496,0.0000046670634,0.000034017314,0.000024216435,0.000029626603],"domain_scores_gemma":[0.99956495,0.000055346853,0.00020869804,0.00003477309,0.00003513353,0.00010112354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014756832,0.00021100877,0.00014512576,0.00093030056,0.00037754758,0.00046321735,0.00024288523,0.00019075931,0.00096420303],"category_scores_gemma":[0.0003199638,0.00019809918,0.00022548749,0.0004040791,0.00026902684,0.0002336635,0.0003437572,0.00029154177,0.00017393228],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046444935,0.00011313328,0.8816606,0.00004932017,0.0001963102,0.0009662662,0.0010111912,0.0012416483,0.09608728,0.0007481338,0.00023567739,0.017226107],"study_design_scores_gemma":[0.000009785056,0.00005700297,0.9967309,0.0000035597584,0.000016608803,0.000406072,0.00014592831,0.0009941115,0.0010939447,0.00008148636,0.00045467739,0.000005857949],"about_ca_topic_score_codex":0.002054288,"about_ca_topic_score_gemma":0.003978172,"teacher_disagreement_score":0.002054288,"about_ca_system_score_codex":0.0002909656,"about_ca_system_score_gemma":0.000068436966,"threshold_uncertainty_score":0.0040846467},"labels":[],"label_agreement":null},{"id":"W1784411555","doi":"10.1088/0004-637x/747/1/59","title":"THE SLOAN DIGITAL SKY SURVEY CO-ADD: A GALAXY PHOTOMETRIC REDSHIFT CATALOG","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Galaxy; Astrophysics; Sky; Redshift; Dark energy; Photometry (optics); Photometric redshift; Cosmology; Astronomy; Large Synoptic Survey Telescope; Estimator; Spectrograph; Observational cosmology; Redshift survey; Spectral line; Statistics; Stars","score_opus":0.012660257687073653,"score_gpt":0.2358399125686723,"score_spread":0.22317965488159863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1784411555","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.043683685,0.0005008142,0.007919008,0.0002695935,0.00009657097,0.0004946751,0.91932225,0.006616386,0.021096917],"genre_scores_gemma":[0.026020573,0.00027590766,0.012975214,0.00011705628,0.00007767037,0.0003789068,0.9541456,0.00075517746,0.005253869],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9988651,0.00011155733,0.00011297895,0.00015477274,0.00061123684,0.00014437678],"domain_scores_gemma":[0.9942531,0.00023509322,0.0012060081,0.0012321012,0.0022949942,0.00077869673],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001128753,0.0010584489,0.00071713567,0.012497288,0.0007846929,0.0008727442,0.00085550925,0.00038748997,0.017566793],"category_scores_gemma":[0.0027817357,0.00041712588,0.00046659447,0.014040479,0.00023348621,0.0009564347,0.0017415979,0.0007970751,0.020835694],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016493007,0.00017773428,0.15001109,0.00048726302,0.0001511023,0.000115541676,0.00025537086,0.0010542164,0.0039711357,0.0021922393,0.75946426,0.081955045],"study_design_scores_gemma":[0.000075021024,0.00004110899,0.37608895,0.00005311159,0.000045100507,0.00019470518,0.00014340677,0.0015261932,0.0022273746,0.00089141086,0.6186666,0.000046993497],"about_ca_topic_score_codex":0.04462031,"about_ca_topic_score_gemma":0.07094899,"teacher_disagreement_score":0.04462031,"about_ca_system_score_codex":0.00095140183,"about_ca_system_score_gemma":0.0020178643,"threshold_uncertainty_score":0.088721156},"labels":[],"label_agreement":null},{"id":"W1784900743","doi":"10.3847/0004-637x/820/1/76","title":"NEUTRINO-DRIVEN CONVECTION IN CORE-COLLAPSE SUPERNOVAE: HIGH-RESOLUTION SIMULATIONS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"Sherman Fairchild Foundation; National Centre for Supercomputing Applications; California Institute of Technology; National Science Foundation","keywords":"Turbulence; Convection; Scaling; Energy cascade; Kinetic energy; Momentum (technical analysis); Energy–momentum relation; Shock wave; Accretion (finance)","score_opus":0.022819945821699338,"score_gpt":0.28427792505279165,"score_spread":0.2614579792310923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1784900743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99019027,0.00016951929,0.0051403954,0.00023320554,0.000028617429,0.00003904666,0.00049440196,0.0002206224,0.003483992],"genre_scores_gemma":[0.99488926,0.000076711134,0.0039605233,0.000061831415,0.00001576786,0.000041480424,0.0005195733,0.00006462751,0.00037009481],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999711,0.00010529446,0.000015874997,0.000032161664,0.00006441864,0.0000711751],"domain_scores_gemma":[0.9982376,0.000988347,0.0001574225,0.00016829817,0.00021501168,0.00023322341],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00085703627,0.00061015657,0.001038216,0.00053019886,0.0006165736,0.0010034182,0.0016674718,0.0013384377,0.0016024505],"category_scores_gemma":[0.0032976717,0.00038791093,0.0008646886,0.00070440164,0.0011331765,0.00060797477,0.0010308606,0.0011359585,0.0001587656],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017955978,0.00016348029,0.0044942466,0.000034521472,0.00006794392,0.000090375004,0.00005574127,0.9910157,0.0015015228,0.0013676803,0.0002196658,0.00080960843],"study_design_scores_gemma":[0.000045310615,0.000030513522,0.0009585258,0.000003865466,0.00000604624,0.000005835388,0.000017198709,0.99823654,0.00031595383,0.00029825713,0.00007667683,0.000005355736],"about_ca_topic_score_codex":0.01761631,"about_ca_topic_score_gemma":0.008655459,"teacher_disagreement_score":0.01761631,"about_ca_system_score_codex":0.0009427727,"about_ca_system_score_gemma":0.0009952802,"threshold_uncertainty_score":0.035027504},"labels":[],"label_agreement":null},{"id":"W1787842274","doi":"10.3847/0004-637x/816/1/34","title":"UV DRIVEN EVAPORATION OF CLOSE-IN PLANETS: ENERGY-LIMITED, RECOMBINATION-LIMITED, AND PHOTON-LIMITED FLOWS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Ionization; Flow (mathematics); Flux (metallurgy); Evaporation; Scaling; Mean free path; Volumetric flow rate; Cooling flow","score_opus":0.016843072742813988,"score_gpt":0.23109560610865326,"score_spread":0.21425253336583927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1787842274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99655604,0.000097612196,0.0014676536,0.00007089042,0.000008188345,0.000009512989,0.00008554369,0.000033399734,0.0016711531],"genre_scores_gemma":[0.99899846,0.000042011834,0.00052245095,0.000018361243,0.0000035283588,0.000007307764,0.00007183112,0.000017683416,0.00031827492],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994516,0.000009562287,0.0000028721327,0.000009682869,0.000010633517,0.00002209395],"domain_scores_gemma":[0.99970824,0.00014380687,0.00005033559,0.000022955137,0.000026104673,0.00004862978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019747892,0.00028691973,0.0005338086,0.00031057379,0.00066251244,0.0006492105,0.0004719927,0.00050882343,0.0013212218],"category_scores_gemma":[0.0010400093,0.00022989478,0.0005618415,0.00022737567,0.00054897193,0.00082979794,0.0006250065,0.00058169954,0.000092625814],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021584384,0.00022790633,0.029683314,0.000115260176,0.00015445332,0.00078294816,0.00026194283,0.9121816,0.04828934,0.004271761,0.00045790416,0.0033577227],"study_design_scores_gemma":[0.00007272008,0.00012762369,0.015276698,0.000013114511,0.000027390786,0.0001366566,0.00015184726,0.9693475,0.0123941805,0.0018011031,0.000621966,0.00002915862],"about_ca_topic_score_codex":0.0027394812,"about_ca_topic_score_gemma":0.0016822394,"teacher_disagreement_score":0.0027394812,"about_ca_system_score_codex":0.00061023136,"about_ca_system_score_gemma":0.0002854673,"threshold_uncertainty_score":0.0054470897},"labels":[],"label_agreement":null},{"id":"W1790289060","doi":"10.1088/0004-637x/804/2/114","title":"PARAMETER ESTIMATION FOR BINARY NEUTRON-STAR COALESCENCES WITH REALISTIC NOISE DURING THE ADVANCED LIGO ERA","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":150,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"LIGO; Gravitational wave; Physics; Sky; Neutron star; Binary number; Noise (video); Chirp; Luminosity distance; Observatory; Astrophysics; Interferometry; Waveform; Redshift; Computer science; Algorithm; Astronomy; Galaxy; Optics; Artificial intelligence; Laser; Mathematics","score_opus":0.01626016541129973,"score_gpt":0.31013768530077274,"score_spread":0.293877519889473,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1790289060","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8871154,0.00068636547,0.10967497,0.00037141226,0.000027921613,0.00001882354,0.00031439614,0.0006404839,0.0011502015],"genre_scores_gemma":[0.9864705,0.00008170541,0.012349756,0.000046098445,0.000017569164,0.000010272758,0.0007471635,0.000060930313,0.00021599243],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99920124,0.00023980973,0.00006633003,0.00023543529,0.00017355458,0.000083648156],"domain_scores_gemma":[0.98776543,0.009543057,0.0011781479,0.0007086534,0.0005173191,0.00028748444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004367874,0.0006162405,0.00069189124,0.00090445194,0.00042042352,0.0013104179,0.00092922687,0.000840746,0.00059252896],"category_scores_gemma":[0.038200483,0.00034650657,0.00042869223,0.0005734944,0.0007007135,0.0012954213,0.0013730034,0.00096154446,0.00021822624],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007110839,0.00007565208,0.13846654,0.00012497639,0.00022402404,0.00034948692,0.00030399094,0.7966866,0.0061462754,0.008763342,0.0008769174,0.04727108],"study_design_scores_gemma":[0.000023655639,0.000039200986,0.017634094,0.000019013007,0.00001748011,0.000090496884,0.000056974142,0.9738696,0.0028949408,0.004901946,0.00042702782,0.000025604202],"about_ca_topic_score_codex":0.00831555,"about_ca_topic_score_gemma":0.004006111,"teacher_disagreement_score":0.00831555,"about_ca_system_score_codex":0.00072142977,"about_ca_system_score_gemma":0.0006674605,"threshold_uncertainty_score":0.02309978},"labels":[],"label_agreement":null},{"id":"W1797834216","doi":"10.1088/0004-637x/744/2/149","title":"THE FAINT-END SLOPE OF THE REDSHIFT 5.7 Lyα LUMINOSITY FUNCTION<sup>,</sup>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Galaxy; Equivalent width; Redshift; Hubble Deep Field; Subaru Telescope; Luminosity function; Field galaxy; Cosmology; Luminosity; Reionization","score_opus":0.010728168503645961,"score_gpt":0.19312779205591504,"score_spread":0.18239962355226907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1797834216","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9621307,0.00032277426,0.008659031,0.00012327051,0.0000227573,0.0000106806265,0.0038238277,0.00036169693,0.02454526],"genre_scores_gemma":[0.9932018,0.00009546199,0.0025580379,0.00003660872,0.000011714091,0.00000498446,0.0024807567,0.000041506064,0.0015690981],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999,0.000011331488,0.0000068432805,0.000032430304,0.000032263943,0.000017089147],"domain_scores_gemma":[0.99886465,0.00021628478,0.0005489717,0.00013546714,0.00014164027,0.0000929667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004027155,0.00021947573,0.00011720353,0.0009894304,0.00013615015,0.00088700466,0.000404441,0.00020112589,0.0048274253],"category_scores_gemma":[0.0012180912,0.000106179294,0.00016837109,0.000572333,0.0002053481,0.00054462557,0.0003271034,0.0002491166,0.0023156868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011955327,0.000027007898,0.93013775,0.000065201515,0.00004374134,0.00020249821,0.00014369204,0.0017210625,0.03313893,0.0039370386,0.0020346,0.028428951],"study_design_scores_gemma":[0.0000017056298,0.000029190378,0.9780096,0.000015830083,0.000017990395,0.000651839,0.0001205923,0.0059840875,0.008940975,0.0009813354,0.005235059,0.000011899547],"about_ca_topic_score_codex":0.00075807236,"about_ca_topic_score_gemma":0.0016178087,"teacher_disagreement_score":0.0048274253,"about_ca_system_score_codex":0.000296494,"about_ca_system_score_gemma":0.00006358413,"threshold_uncertainty_score":0.016149402},"labels":[],"label_agreement":null},{"id":"W1807725900","doi":"10.1088/0004-637x/815/2/103","title":"DENSE GAS FRACTION AND STAR FORMATION EFFICIENCY VARIATIONS IN THE ANTENNAE GALAXIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Science Council; Deutsche Forschungsgemeinschaft; National Institutes of Natural Sciences; California Institute of Technology; Gordon and Betty Moore Foundation; National Science Foundation; James S. McDonnell Foundation; National Radio Astronomy Observatory","keywords":"Star formation; Galaxy; Millimeter; Line (geometry); Spectral line; Infrared; Emission spectrum; Luminous infrared galaxy; Optical depth","score_opus":0.011997888952855548,"score_gpt":0.2228148013894112,"score_spread":0.21081691243655565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1807725900","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99936074,0.000025093641,0.00005967659,0.0000049627656,3.3147273e-7,0.0000013327226,0.00019871246,0.000009714568,0.00033939537],"genre_scores_gemma":[0.99954385,0.000011791229,0.000095060204,0.0000026232246,0.0000013008402,0.0000015246845,0.00024735898,0.0000024340052,0.00009396669],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998647,0.000020743346,0.000006204059,0.00005844006,0.000019394649,0.000030484256],"domain_scores_gemma":[0.9993894,0.0001003739,0.00022285857,0.00009115932,0.00006864426,0.00012747444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017676115,0.00014142011,0.0001518292,0.0010816024,0.00012856601,0.00040825867,0.00017853803,0.00017048024,0.00074645004],"category_scores_gemma":[0.00069907133,0.00014380034,0.00012246595,0.0006514793,0.00026040955,0.00023965168,0.00026297668,0.00011927081,0.00022229996],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006461214,0.000017531362,0.9849941,0.00000451499,0.00003825617,0.0000459092,0.00017463787,0.00038972351,0.011479901,0.00008006867,0.0000792554,0.002631388],"study_design_scores_gemma":[0.0000012440511,0.000010513157,0.9992698,4.4813137e-7,0.000003422281,0.00003495357,0.00003397127,0.00024074441,0.0003062431,0.000013941995,0.00008325738,0.000001437549],"about_ca_topic_score_codex":0.005000538,"about_ca_topic_score_gemma":0.0060600433,"teacher_disagreement_score":0.005000538,"about_ca_system_score_codex":0.00030596615,"about_ca_system_score_gemma":0.00005338747,"threshold_uncertainty_score":0.00994283},"labels":[],"label_agreement":null},{"id":"W1812305348","doi":"10.1086/339261","title":"Dissecting the Luminosity Function of the Coma Cluster of Galaxies Using Canada‐France‐Hawaii Telescope1 Wide‐Field Images","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Coma Cluster; Luminosity function; Galaxy; Coma (optics); Luminosity; Cluster (spacecraft)","score_opus":0.007715444981505394,"score_gpt":0.1928420687011638,"score_spread":0.1851266237196584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1812305348","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939237,0.0001472343,0.0012050873,0.000051180854,0.000003812966,0.000012397005,0.0006492148,0.0000920386,0.003915279],"genre_scores_gemma":[0.9956292,0.00010564811,0.0016193021,0.000022033648,0.000007570861,0.0000065462323,0.0009062271,0.00002641311,0.001677076],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999473,0.0000033581716,0.000001263597,0.000012020938,0.000012014405,0.000023952109],"domain_scores_gemma":[0.999701,0.000050895593,0.000032576034,0.00001507116,0.00008851151,0.00011199771],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016376798,0.00022615043,0.00012295999,0.001837312,0.0004665391,0.00065737666,0.00026432503,0.00023349933,0.002467045],"category_scores_gemma":[0.00033675757,0.00019057753,0.00020172876,0.0009054663,0.00014589359,0.0002650905,0.00030097683,0.00019479437,0.0003696298],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054266996,0.000074595664,0.46747744,0.00011449476,0.00019892328,0.0008226966,0.0017977162,0.004081308,0.4579938,0.0015032791,0.0038389845,0.06155414],"study_design_scores_gemma":[0.0000044477033,0.000013472915,0.993543,0.0000043558243,0.00002054104,0.000083401006,0.00016667426,0.0016044368,0.0036920845,0.000057371046,0.00080034084,0.000009889933],"about_ca_topic_score_codex":0.14011833,"about_ca_topic_score_gemma":0.23199862,"teacher_disagreement_score":0.14011833,"about_ca_system_score_codex":0.0009506363,"about_ca_system_score_gemma":0.00040157174,"threshold_uncertainty_score":0.27860552},"labels":[],"label_agreement":null},{"id":"W1813160828","doi":"10.3847/0004-637x/821/1/56","title":"SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. III. OPTICAL CONTINUUM EMISSION AND BROADBAND TIME DELAYS IN NGC 5548","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":310,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Natural Sciences and Engineering Research Council of Canada; University of California, Santa Barbara; Jet Propulsion Laboratory; National Research Foundation of Korea; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Space Telescope Science Institute; American Academy in Rome; Science and Technology Facilities Council; National Research Foundation; David and Lucile Packard Foundation; Ministry of Science, ICT and Future Planning; Ohio State University; Howard Hughes Medical Institute; Danmarks Grundforskningsfond; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Georgia State University; California Institute of Technology; National Aeronautics and Space Administration; Danmarks Frie Forskningsfond; National Science Foundation","keywords":"Physics; Astrophysics; Wavelength; Algorithm; Optics; Computer science","score_opus":0.010278538560239631,"score_gpt":0.22566826626977468,"score_spread":0.21538972770953504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1813160828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9765287,0.00015971207,0.0020215942,0.00020093782,0.000032808894,0.00006020086,0.01351051,0.00059737585,0.0068881786],"genre_scores_gemma":[0.9478649,0.00011411513,0.0067879744,0.00011445584,0.000045752327,0.000105646795,0.036481097,0.00018015398,0.008305969],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981827,0.00002233254,0.000009148491,0.000047627625,0.00004812007,0.00005442743],"domain_scores_gemma":[0.9994118,0.000038729468,0.00014868897,0.00015127567,0.00011109409,0.00013847365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042814028,0.00033671694,0.00018651524,0.00094681536,0.0003114779,0.00039770454,0.00036421558,0.0002077438,0.0037506677],"category_scores_gemma":[0.00067155715,0.00014148135,0.0001828646,0.00044862513,0.00012313,0.0002729659,0.00041892985,0.00021436447,0.0016945573],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011472931,0.00035377304,0.7826917,0.00007784595,0.00012481316,0.0008018079,0.0010005342,0.002560752,0.05984268,0.0007728168,0.025567856,0.1250582],"study_design_scores_gemma":[0.000045043253,0.00011481255,0.9800166,0.000008176556,0.000024228808,0.00019321928,0.00009303765,0.0013554641,0.003762651,0.00012957539,0.014249178,0.000008106615],"about_ca_topic_score_codex":0.017872686,"about_ca_topic_score_gemma":0.025693981,"teacher_disagreement_score":0.017872686,"about_ca_system_score_codex":0.00044027204,"about_ca_system_score_gemma":0.00022658124,"threshold_uncertainty_score":0.035537302},"labels":[],"label_agreement":null},{"id":"W1813180485","doi":"10.3847/0004-637x/816/2/80","title":"THE SEGUE K GIANT SURVEY. III. QUANTIFYING GALACTIC HALO SUBSTRUCTURE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Halo; Physics; Astrophysics; Metallicity; Substructure; Milky Way; Galactic halo; Stars; Astronomy; Galaxy","score_opus":0.022982899384159212,"score_gpt":0.24755977661824052,"score_spread":0.22457687723408132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1813180485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9816465,0.0004956295,0.00021280094,0.000065726046,0.0000067271117,0.000010564768,0.016125334,0.00010505446,0.0013316934],"genre_scores_gemma":[0.9648841,0.0002417773,0.00068417157,0.000044096807,0.000012686903,0.000016798667,0.033098087,0.00004024959,0.0009780902],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997869,0.00004691553,0.000013245546,0.00006279658,0.000044396504,0.00004568051],"domain_scores_gemma":[0.9992955,0.000057603804,0.00025832636,0.000113101814,0.00014031747,0.00013511402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042519174,0.00026427966,0.00020515981,0.0019318288,0.00020341242,0.00043022394,0.00026950872,0.0002580047,0.0009937311],"category_scores_gemma":[0.0010840322,0.00011331928,0.00031593168,0.0020758219,0.00017077781,0.00030410144,0.0007594086,0.00012519956,0.00081091456],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012255745,0.000008463484,0.9891115,0.000050478648,0.00017535134,0.000053462307,0.00015947704,0.0003942212,0.0013307243,0.00009781734,0.0024602045,0.006035687],"study_design_scores_gemma":[0.0000056356103,0.00001413572,0.9971961,0.0000072561274,0.000016039285,0.000044629094,0.00018607326,0.00033667238,0.00020365448,0.000031150103,0.001955471,0.0000030911947],"about_ca_topic_score_codex":0.03186441,"about_ca_topic_score_gemma":0.055412866,"teacher_disagreement_score":0.03186441,"about_ca_system_score_codex":0.000358692,"about_ca_system_score_gemma":0.00019666116,"threshold_uncertainty_score":0.06335789},"labels":[],"label_agreement":null},{"id":"W1814292902","doi":"10.1088/0004-637x/812/1/7","title":"THE THREE-mm ULTIMATE MOPRA MILKY WAY SURVEY. II. CLOUD AND STAR FORMATION NEAR THE FILAMENTARY MINISTARBURST RCW 106","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Star formation; Cloud computing; Star (game theory); Molecular cloud; Stellar evolution","score_opus":0.022503905914302735,"score_gpt":0.2500997556315045,"score_spread":0.22759584971720176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1814292902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93870336,0.00050523155,0.00039332165,0.0011346054,0.00003075279,0.00004077305,0.04599347,0.00012984418,0.0130686285],"genre_scores_gemma":[0.94113064,0.00030871519,0.001773116,0.00022127866,0.000045311703,0.000057911788,0.0487581,0.0000506246,0.0076543433],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998771,0.00001327555,0.000008986911,0.000031435527,0.000035423654,0.000033831253],"domain_scores_gemma":[0.99954706,0.000026677279,0.00012780497,0.000051574687,0.0000857943,0.00016106771],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027522794,0.00008190144,0.00013433378,0.0013201224,0.00038726008,0.00048939855,0.00027786163,0.00029804086,0.0016299093],"category_scores_gemma":[0.00066899235,0.00012715672,0.00017701939,0.0011792863,0.00011498468,0.00040977853,0.0009764703,0.00021654734,0.0006617448],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015043598,0.00003052989,0.95381224,0.00004574036,0.0000649576,0.00016158984,0.00037332816,0.00033710073,0.0031916057,0.0008892058,0.015197909,0.025745407],"study_design_scores_gemma":[0.000005595332,0.0000063683024,0.991405,0.000006743018,0.0000055537425,0.000033253917,0.00013250668,0.00013605322,0.00011435532,0.0000680933,0.008084715,0.0000018246953],"about_ca_topic_score_codex":0.070050575,"about_ca_topic_score_gemma":0.18620396,"teacher_disagreement_score":0.070050575,"about_ca_system_score_codex":0.0004883433,"about_ca_system_score_gemma":0.00062911486,"threshold_uncertainty_score":0.13928568},"labels":[],"label_agreement":null},{"id":"W1814416524","doi":"10.1088/0004-637x/809/1/74","title":"OGLE-2012-BLG-0563Lb: A SATURN-MASS PLANET AROUND AN M DWARF WITH THE MASS CONSTRAINED BY<i>SUBARU</i>AO IMAGING","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Institutes of Natural Sciences; Narodowym Centrum Nauki; National Research Foundation of Korea; Chinese Academy of Sciences; Royal Society Te Apārangi; Qatar Foundation; Qatar National Research Fund; National Research Foundation; Science and Technology Facilities Council; California NanoSystems Institute; National Astronomical Observatory of Japan; European Commission; Japan Society for the Promotion of Science","keywords":"Physics; Gravitational microlensing; Planet; Astrophysics; Exoplanet; Astronomy; Planetary system; Brown dwarf; Subaru Telescope; Transit (satellite); Planetary mass; Stellar mass; Galaxy; Spectrograph; Star formation","score_opus":0.010704885168073625,"score_gpt":0.2159609029246173,"score_spread":0.20525601775654367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1814416524","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970607,0.00035485558,0.00038150043,0.000099724115,0.000016146634,0.000007600555,0.00031512216,0.000062779196,0.0017014827],"genre_scores_gemma":[0.9978928,0.000064820015,0.00054577866,0.000079271056,0.000016303795,0.0000021977464,0.0006372249,0.000009778111,0.00075178774],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99990845,0.000004307343,0.0000060417024,0.00003440287,0.000020723766,0.000026006419],"domain_scores_gemma":[0.9997781,0.0000090567755,0.000075695905,0.000022411075,0.000014336782,0.000100480574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013638767,0.0003203737,0.00035598222,0.0005937636,0.0005962137,0.0005238731,0.0003174643,0.00084992533,0.0010244484],"category_scores_gemma":[0.00016978172,0.00016516147,0.00020141625,0.00036224682,0.00028419885,0.00034797768,0.00078830565,0.00043193114,0.0011926327],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010998665,0.00033179784,0.37197083,0.00024457715,0.00011372029,0.03419419,0.0008590089,0.00037795384,0.56041837,0.00075384945,0.0019922599,0.02764366],"study_design_scores_gemma":[0.000057292506,0.0009526448,0.89789313,0.000038432103,0.00008448964,0.0380198,0.000637474,0.0014899817,0.047184218,0.0005020013,0.013106126,0.000034338424],"about_ca_topic_score_codex":0.0016380996,"about_ca_topic_score_gemma":0.0027014846,"teacher_disagreement_score":0.0016380996,"about_ca_system_score_codex":0.00031491678,"about_ca_system_score_gemma":0.000113768496,"threshold_uncertainty_score":0.0034271479},"labels":[],"label_agreement":null},{"id":"W1817897403","doi":"10.1088/0004-637x/794/1/72","title":"ISOCHRONES FOR OLD (&gt;5 GYR) STARS AND STELLAR POPULATIONS. I. MODELS FOR –2.4 ⩽ [Fe/H] ⩽+0.6, 0.25 ⩽<i>Y</i>⩽ 0.33, AND –0.4 ⩽ [α/Fe] ⩽+0.4","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Regina; University of Victoria","funders":"","keywords":"Globular cluster; Open cluster; Stars; Helium; Cluster (spacecraft); Pleiades; Star cluster; Stellar evolution; Subdwarf","score_opus":0.020642059124329856,"score_gpt":0.24151658609108664,"score_spread":0.2208745269667568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1817897403","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.27281335,0.0029343679,0.3422494,0.00077692413,0.0014837075,0.0010063441,0.19053411,0.04805758,0.14014418],"genre_scores_gemma":[0.5901853,0.0014946887,0.20165135,0.00032248299,0.00013126625,0.0013841282,0.16172613,0.0071046404,0.035999928],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986076,0.000023328483,0.000007788417,0.000054368316,0.000030747906,0.000023016428],"domain_scores_gemma":[0.99954396,0.00006742238,0.000075858174,0.00011136848,0.00014775878,0.000053509477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061395095,0.000625595,0.00027733468,0.0010008157,0.0004459069,0.0009723044,0.0010385836,0.0006720075,0.024531644],"category_scores_gemma":[0.0016480467,0.00045098853,0.0008950914,0.0007715722,0.00030130844,0.00074819796,0.0004705283,0.0011949462,0.018691579],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012115048,0.0004768944,0.18305123,0.0013350176,0.0005071738,0.00035304952,0.0025064307,0.24660796,0.032800443,0.09128016,0.2966149,0.14325525],"study_design_scores_gemma":[0.00023443026,0.00036135165,0.22845885,0.0002148645,0.0002715471,0.0007616784,0.00043421992,0.16669081,0.012640219,0.02111944,0.56863165,0.00018091126],"about_ca_topic_score_codex":0.007218343,"about_ca_topic_score_gemma":0.01090706,"teacher_disagreement_score":0.024531644,"about_ca_system_score_codex":0.0011129667,"about_ca_system_score_gemma":0.0005372838,"threshold_uncertainty_score":0.08206648},"labels":[],"label_agreement":null},{"id":"W1822769209","doi":"10.1088/0004-637x/806/1/128","title":"SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. I. ULTRAVIOLET OBSERVATIONS OF THE SEYFERT 1 GALAXY NGC 5548 WITH THE COSMIC ORIGINS SPECTROGRAPH ON<i>HUBBLE SPACE TELESCOPE</i>","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":170,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Natural Sciences and Engineering Research Council of Canada; University of California, Santa Barbara; Jet Propulsion Laboratory; Space Telescope Science Institute; American Academy in Rome; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Georgia State University; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Science and Technology Facilities Council; National Research Foundation; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; California Institute of Technology; Ohio State University; Danmarks Frie Forskningsfond; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Space Telescope Imaging Spectrograph; Galaxy; Emission spectrum; Reverberation mapping; Spectrograph; Active galactic nucleus; Hubble space telescope; Spectral line","score_opus":0.016853724210129293,"score_gpt":0.22026001085507182,"score_spread":0.20340628664494254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1822769209","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89078635,0.00059873983,0.0062811365,0.0009086877,0.00018781377,0.0008859714,0.07462133,0.00086141925,0.02486851],"genre_scores_gemma":[0.7813527,0.00033149845,0.032458782,0.0005536254,0.0001856738,0.0005944517,0.1612218,0.00023132394,0.023070207],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993773,0.0001315769,0.000020837817,0.00013555786,0.00018808342,0.00014659732],"domain_scores_gemma":[0.99840266,0.00008029515,0.00027223458,0.00032019522,0.00033277003,0.00059185096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014185423,0.000765942,0.00029169887,0.0011206687,0.0005184577,0.0004241788,0.00050322333,0.00033931847,0.004352016],"category_scores_gemma":[0.0006972153,0.00018335435,0.00022046253,0.00068732165,0.00031365323,0.000494961,0.0008353453,0.00045893347,0.0019671172],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0048670135,0.0015013153,0.6673847,0.00024466263,0.0003303122,0.001414933,0.002014862,0.0015175203,0.06688743,0.002964881,0.0583673,0.19250506],"study_design_scores_gemma":[0.00027138265,0.00083136396,0.9339579,0.000015824635,0.00006125114,0.00035606197,0.00021217822,0.0007695069,0.006965869,0.00037962905,0.05616259,0.000016365406],"about_ca_topic_score_codex":0.014449415,"about_ca_topic_score_gemma":0.01980494,"teacher_disagreement_score":0.014449415,"about_ca_system_score_codex":0.0007142053,"about_ca_system_score_gemma":0.000785273,"threshold_uncertainty_score":0.02873063},"labels":[],"label_agreement":null},{"id":"W1827437670","doi":"10.1088/0004-637x/810/1/76","title":"NLTE AND LTE LICK INDICES FOR RED GIANTS FROM [Fe/H] 0.0 TO −6.0 AT SDSS AND IDS SPECTRAL RESOLUTION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Metallicity; Luminosity; Stars; Spectral resolution; Giant star; Spectral line; Red giant","score_opus":0.01448349577660788,"score_gpt":0.2316093995818614,"score_spread":0.21712590380525354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1827437670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99450195,0.00006527677,0.0002726496,0.0000304554,0.0000018764307,0.0000021075093,0.0023866424,0.000096274285,0.002642841],"genre_scores_gemma":[0.99211955,0.000028742701,0.00025274974,0.000022782364,0.0000029776882,0.0000051540887,0.0068941643,0.00002087595,0.0006529748],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998721,0.000011474191,0.000009814228,0.00003232781,0.000025525063,0.00004885112],"domain_scores_gemma":[0.99921024,0.00013750045,0.00016785724,0.00010664793,0.00018594567,0.00019176224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031344665,0.00016482921,0.00022321365,0.0013254591,0.00024960065,0.00062860124,0.00024065435,0.0002598245,0.001946871],"category_scores_gemma":[0.0013972983,0.0001340983,0.0002198012,0.00089417427,0.00023144444,0.00044953864,0.0006196735,0.00016828779,0.00065789284],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004055402,0.000046520494,0.96381783,0.000058226757,0.00010331649,0.00009881919,0.00035419577,0.00594254,0.012274561,0.0011557929,0.0024126656,0.013329904],"study_design_scores_gemma":[0.0000072558796,0.00001577602,0.9914072,0.000008699046,0.000013850036,0.00007890719,0.00014954388,0.0051992475,0.0013502879,0.0002293274,0.0015300156,0.000009814995],"about_ca_topic_score_codex":0.006901426,"about_ca_topic_score_gemma":0.012531335,"teacher_disagreement_score":0.006901426,"about_ca_system_score_codex":0.00050600397,"about_ca_system_score_gemma":0.00016856626,"threshold_uncertainty_score":0.013722479},"labels":[],"label_agreement":null},{"id":"W1830023397","doi":"10.1086/322511","title":"The Supernova Remnant G106.3+2.7 and Its Pulsar‐Wind Nebula: Relics of Triggered Star Formation in a Complex Environment","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Pulsar; Nebula; Supernova remnant; Astrophysics; Supernova; Astronomy; Pulsar wind nebula; Near-Earth supernova; Stars","score_opus":0.01705850629976833,"score_gpt":0.22234593818842954,"score_spread":0.20528743188866122,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1830023397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99682426,0.00034103557,0.00044523182,0.000051907547,0.0000068003915,0.000005017796,0.000038144357,0.000025472216,0.0022621746],"genre_scores_gemma":[0.99850464,0.00021826694,0.0003523601,0.000027109347,0.0000129893815,0.0000039772017,0.00019119876,0.0000078352095,0.000681605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999212,0.0000115404255,0.0000049460577,0.000021650809,0.000021565455,0.000019177656],"domain_scores_gemma":[0.99975353,0.000033201028,0.000091803435,0.000035917226,0.00001532483,0.00007025937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018974293,0.00017161752,0.000256086,0.00039050574,0.00056456495,0.0011030535,0.00034954905,0.0004892008,0.001407896],"category_scores_gemma":[0.00041345856,0.00021797836,0.00021477816,0.00036771258,0.00081680267,0.0006196975,0.0014288519,0.00030093812,0.0003612784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089958904,0.0003218722,0.6503205,0.00030951994,0.00025680423,0.040975317,0.004009332,0.005519924,0.21351872,0.033982024,0.0013108106,0.048575666],"study_design_scores_gemma":[0.000077555545,0.0003570223,0.9238373,0.000056405966,0.00012358333,0.031240454,0.0011670336,0.0036939408,0.00789482,0.011978479,0.019510204,0.00006319928],"about_ca_topic_score_codex":0.0007946369,"about_ca_topic_score_gemma":0.00068987015,"teacher_disagreement_score":0.001407896,"about_ca_system_score_codex":0.00019947086,"about_ca_system_score_gemma":0.0002547758,"threshold_uncertainty_score":0.00470984},"labels":[],"label_agreement":null},{"id":"W1831433017","doi":"10.3847/0004-637x/821/2/119","title":"A DEEP SEARCH FOR PROMPT RADIO EMISSION FROM THERMONUCLEAR SUPERNOVAE WITH THE VERY LARGE ARRAY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Jansky; Supernova; Thermonuclear fusion; Stars; Maser; Radio astronomy","score_opus":0.010515421975111601,"score_gpt":0.22449661284203526,"score_spread":0.21398119086692366,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1831433017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9891045,0.0006044187,0.0037941113,0.00010595623,0.000024031338,0.000022287672,0.0011600571,0.00015396146,0.0050307615],"genre_scores_gemma":[0.9931272,0.00017502313,0.003982923,0.00014472338,0.0000502522,0.000013082618,0.0015722623,0.000021557025,0.0009129974],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978095,0.000029665085,0.000012523608,0.00008613734,0.000043815566,0.000046854933],"domain_scores_gemma":[0.99948716,0.00006929004,0.000116210846,0.00008256079,0.00005177986,0.00019301237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048226828,0.00021717428,0.0002230639,0.0012029519,0.0002805141,0.00075678434,0.0002723342,0.00026404872,0.0010398775],"category_scores_gemma":[0.00045130352,0.00019204045,0.00023195473,0.00070495025,0.00023948241,0.00031815996,0.00083355315,0.00032459394,0.0003272372],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004119327,0.00016334128,0.61448586,0.00009132753,0.00019579001,0.00071060593,0.00036299307,0.00085871224,0.31661582,0.0015412802,0.0025290374,0.062033247],"study_design_scores_gemma":[0.000018711695,0.00018724093,0.97762007,0.000014210027,0.00006611299,0.0009104519,0.0001793441,0.0015640963,0.0111979,0.00062152237,0.0075950804,0.00002523672],"about_ca_topic_score_codex":0.0009793004,"about_ca_topic_score_gemma":0.0024425373,"teacher_disagreement_score":0.0012029519,"about_ca_system_score_codex":0.00019319807,"about_ca_system_score_gemma":0.00019041677,"threshold_uncertainty_score":0.0034787655},"labels":[],"label_agreement":null},{"id":"W1839606263","doi":"10.1088/0004-637x/808/1/19","title":"THE MEGASECOND<i>CHANDRA</i>X-RAY VISIONARY PROJECT OBSERVATION OF NGC 3115. II. PROPERTIES OF POINT SOURCES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Astrophysics; Luminosity; Galaxy; Black hole (networking); Neutron star; Astronomy; Spectral line; Erg; Optics","score_opus":0.035735856138388776,"score_gpt":0.2391727153491721,"score_spread":0.2034368592107833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1839606263","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932446,0.00025617075,0.0009930753,0.00002890867,0.0000062023214,0.000025632311,0.0014549139,0.0000647467,0.0039257924],"genre_scores_gemma":[0.9950781,0.000110573215,0.0017683653,0.000017444077,0.000007098718,0.000010724931,0.0022585834,0.0000103897555,0.00073862454],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985766,0.00001248543,0.000007093929,0.000040457344,0.00004273249,0.000039409275],"domain_scores_gemma":[0.9997149,0.000024793948,0.00009521621,0.00003699647,0.00003362725,0.000094493065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002465004,0.00016231938,0.0001749901,0.0010693911,0.00045679114,0.0003523217,0.0002951701,0.00016612478,0.0018033553],"category_scores_gemma":[0.00031110097,0.00012745048,0.00017966326,0.0008977789,0.00017777056,0.00032887634,0.00041929403,0.00020142933,0.00031721077],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052189257,0.00014773366,0.8521053,0.00018605546,0.00010151534,0.00087325025,0.00066089554,0.0011554882,0.09438587,0.0009711822,0.0025358186,0.046355024],"study_design_scores_gemma":[0.000003988904,0.000056337416,0.99596786,0.0000062727822,0.000011272664,0.0004042008,0.000054142027,0.000265108,0.001564835,0.000055601147,0.0016053262,0.0000051083657],"about_ca_topic_score_codex":0.0075313603,"about_ca_topic_score_gemma":0.024345635,"teacher_disagreement_score":0.0075313603,"about_ca_system_score_codex":0.00037006597,"about_ca_system_score_gemma":0.00030265583,"threshold_uncertainty_score":0.014975071},"labels":[],"label_agreement":null},{"id":"W1842313348","doi":"10.1088/0004-637x/762/1/10","title":"THE ATACAMA COSMOLOGY TELESCOPE: DATA CHARACTERIZATION AND MAPMAKING","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"SLAC National Accelerator Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; University of Toronto; Fondo de Financiamiento de Centros de Investigación en Áreas Prioritarias; Science and Technology Facilities Council; Centro de Astrofísica y Tecnologías Afines; Government of Ontario; National Science Foundation; Compute Canada; University of Pennsylvania; Princeton University; U.S. Department of Energy","keywords":"Physics; Cosmology; Astronomy; Telescope; Astrophysics; Observational cosmology; Characterization (materials science); Dark energy","score_opus":0.015403130198196033,"score_gpt":0.23732768250520436,"score_spread":0.22192455230700833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1842313348","genre_codex":"dataset","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.12381044,0.0029384778,0.12540732,0.006047274,0.0008653439,0.0019600785,0.45329374,0.04502883,0.24064843],"genre_scores_gemma":[0.24588598,0.0014799013,0.28901312,0.00083712797,0.0004503804,0.001411958,0.41532066,0.009163054,0.036437795],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9981444,0.0002679017,0.00015683046,0.00034965805,0.00091960054,0.00016161897],"domain_scores_gemma":[0.99185705,0.00061949715,0.0005653211,0.002784526,0.003082107,0.0010915073],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032174566,0.00043383328,0.000484679,0.0064080553,0.001730214,0.0034153424,0.001517562,0.0006877184,0.011613684],"category_scores_gemma":[0.009495646,0.00046007056,0.00040323066,0.010451659,0.0005444968,0.0032792434,0.0024789907,0.0011871646,0.008769218],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031852812,0.00018587716,0.066702865,0.00042444284,0.00011475765,0.00022488115,0.003056475,0.0019469853,0.015039659,0.013186829,0.39408854,0.50471014],"study_design_scores_gemma":[0.00005864743,0.000019052564,0.08984461,0.00011450437,0.000023628772,0.0001494782,0.001200604,0.0047292667,0.0061078463,0.007167681,0.89052033,0.000064262254],"about_ca_topic_score_codex":0.05669677,"about_ca_topic_score_gemma":0.05443293,"teacher_disagreement_score":0.05669677,"about_ca_system_score_codex":0.00141887,"about_ca_system_score_gemma":0.0054196874,"threshold_uncertainty_score":0.11273354},"labels":[],"label_agreement":null},{"id":"W1844787056","doi":"10.1088/0004-637x/806/2/181","title":"WATER ICE LINES AND THE FORMATION OF GIANT MOONS AROUND SUPER-JOVIAN PLANETS","year":2015,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada; McMaster University","keywords":"Jovian; Exoplanet; Icy moon; Physics; Astrobiology; Planet; Astronomy; Jupiter (rocket family); Gas giant; Galilean moons; Astrophysics; Natural satellite; Saturn; Space exploration","score_opus":0.01580417435751822,"score_gpt":0.22190678017850088,"score_spread":0.20610260582098267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1844787056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980737,0.00005652684,0.0006375823,0.000030533545,0.000006388434,0.0000054151174,0.000056828285,0.000015831474,0.0011171898],"genre_scores_gemma":[0.99931085,0.000039333332,0.00035719946,0.000007076742,0.0000015109213,0.000004486709,0.00005550683,0.0000069786383,0.00021707443],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999615,0.000008196511,0.0000019428098,0.0000056256113,0.0000061971846,0.000016583735],"domain_scores_gemma":[0.9998258,0.00005941916,0.00005332652,0.000011686085,0.000016300937,0.000033580793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009032404,0.00023280688,0.00019764224,0.00023113724,0.00028985256,0.00044211646,0.00036587,0.00038664314,0.001547262],"category_scores_gemma":[0.000502776,0.00014118527,0.00039001115,0.00016246617,0.0004008892,0.0003868734,0.00036388118,0.00022359706,0.000097361866],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023079329,0.00015595953,0.07867364,0.00006808587,0.00010188628,0.00051490194,0.00016991067,0.8991966,0.014594669,0.00191204,0.00030927116,0.004072232],"study_design_scores_gemma":[0.000198745,0.0004883965,0.07465067,0.000023939147,0.00008785258,0.00019636343,0.00049055426,0.9146767,0.0054297084,0.0020343366,0.001695553,0.00002717114],"about_ca_topic_score_codex":0.006166773,"about_ca_topic_score_gemma":0.004385781,"teacher_disagreement_score":0.006166773,"about_ca_system_score_codex":0.00026665197,"about_ca_system_score_gemma":0.00024108174,"threshold_uncertainty_score":0.012261808},"labels":[],"label_agreement":null},{"id":"W1852006159","doi":"10.1088/0004-637x/808/1/20","title":"THE MEGASECOND<i>CHANDRA</i>X-RAY VISIONARY PROJECT OBSERVATION OF NGC 3115. III. LUMINOSITY FUNCTIONS OF LMXBS AND DEPENDENCE ON STELLAR ENVIRONMENTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Luminosity; Physics; Astrophysics; Astronomy; X-ray; Galaxy; Optics","score_opus":0.02571063950141276,"score_gpt":0.23735399929742465,"score_spread":0.2116433597960119,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1852006159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952832,0.00017739249,0.00091302826,0.000028927643,0.0000050604394,0.000011038847,0.0013525068,0.0000859729,0.0021427355],"genre_scores_gemma":[0.9958442,0.00006916625,0.0016955578,0.000023449116,0.0000060546463,0.0000085011825,0.0019204909,0.00001705138,0.0004156055],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999884,0.0000106049965,0.0000052856935,0.000036046556,0.000028334876,0.00003569053],"domain_scores_gemma":[0.9996712,0.000039723156,0.00009599303,0.000049507125,0.000037578582,0.00010593983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025590393,0.00022456986,0.0001587877,0.00098009,0.00032459767,0.0003594994,0.00026171803,0.00018490125,0.0011263281],"category_scores_gemma":[0.0003428944,0.00016840045,0.00026029933,0.0007082627,0.00017385518,0.00029790335,0.00031857972,0.0002854205,0.0002014055],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004227726,0.00009287994,0.8600509,0.00013745525,0.0001339101,0.00053515483,0.00042011673,0.0018535182,0.10980852,0.0007864361,0.0019922506,0.023766031],"study_design_scores_gemma":[0.0000030984388,0.00002532414,0.9967706,0.0000044034427,0.000010188634,0.0001607561,0.000025088684,0.00060140615,0.0016842525,0.000037632413,0.00067305594,0.000004269005],"about_ca_topic_score_codex":0.008557267,"about_ca_topic_score_gemma":0.02209078,"teacher_disagreement_score":0.008557267,"about_ca_system_score_codex":0.0003978014,"about_ca_system_score_gemma":0.00018101292,"threshold_uncertainty_score":0.01701492},"labels":[],"label_agreement":null},{"id":"W1852220742","doi":"10.1088/0004-637x/807/2/150","title":"230 GHz VLBI OBSERVATIONS OF M87: EVENT‐HORIZON‐SCALE STRUCTURE DURING AN ENHANCED VERY‐HIGH‐ENERGY $\\gamma $‐RAY STATE IN 2012","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Army Research Office; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Industry Canada; Academia Sinica; National Science Foundation; Government of Canada; Smithsonian Astrophysical Observatory; Gordon and Betty Moore Foundation; Japan Society for the Promotion of Science; Ministry of Education, Culture, Sports, Science and Technology","keywords":"Very-long-baseline interferometry; Physics; Astrophysics; Event horizon; Brightness; Flux (metallurgy); Angular diameter; Radio telescope; Astronomy; Event (particle physics); Stars","score_opus":0.010106052361636366,"score_gpt":0.2189503091077061,"score_spread":0.20884425674606974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1852220742","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99351716,0.0001638409,0.00020992816,0.0002731631,0.000014786477,0.0000047096014,0.0008858558,0.00003133218,0.004899255],"genre_scores_gemma":[0.9979746,0.0000511564,0.00012226784,0.000041859326,0.000012086383,0.000004392963,0.00093271944,0.0000073297138,0.0008536274],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999941,0.000005260799,0.0000017393797,0.000011328733,0.000015202896,0.000025317448],"domain_scores_gemma":[0.9998903,0.00001072007,0.000029939945,0.000010738488,0.000026111815,0.00003219401],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012505136,0.0000731,0.00012283085,0.0005075688,0.00034370853,0.0005838074,0.00015142914,0.0003222552,0.0010881065],"category_scores_gemma":[0.00037681186,0.00009741072,0.00008001304,0.00048570507,0.00019339306,0.00027049953,0.0004969242,0.00034554233,0.0002556418],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010937321,0.0003731716,0.86245984,0.00008618306,0.00022367833,0.0010986602,0.003698817,0.0021500466,0.060195986,0.0037886917,0.014070591,0.05076057],"study_design_scores_gemma":[0.0000034078405,0.000010085867,0.99489766,0.0000058789738,0.000009872036,0.000041805713,0.00021099816,0.00037500856,0.0004306452,0.00012316315,0.0038878683,0.0000036540437],"about_ca_topic_score_codex":0.026446462,"about_ca_topic_score_gemma":0.07509027,"teacher_disagreement_score":0.026446462,"about_ca_system_score_codex":0.0005211142,"about_ca_system_score_gemma":0.0003196418,"threshold_uncertainty_score":0.052585065},"labels":[],"label_agreement":null},{"id":"W1854797695","doi":"10.1088/0004-637x/808/1/70","title":"NEUTRINO-DRIVEN TURBULENT CONVECTION AND STANDING ACCRETION SHOCK INSTABILITY IN THREE-DIMENSIONAL CORE-COLLAPSE SUPERNOVAE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Physics; Convection; Supernova; Neutrino; Instability; Turbulence; Mechanics; Accretion (finance); Astrophysics; Nuclear physics","score_opus":0.027660348713648253,"score_gpt":0.2505732756351366,"score_spread":0.22291292692148834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1854797695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972465,0.000036813868,0.0012094955,0.000091052214,0.000010996938,0.000013289581,0.00008988387,0.000047884736,0.0012540364],"genre_scores_gemma":[0.9982285,0.000032465512,0.0014042099,0.000039454553,0.000006007005,0.000013979578,0.000102956976,0.000018552619,0.00015396737],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998522,0.000039327588,0.00001124678,0.000018749148,0.000032398708,0.00004604258],"domain_scores_gemma":[0.99919015,0.00027919048,0.00017622905,0.00007124549,0.00008661959,0.0001965666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047478455,0.0005384237,0.00052087114,0.00051540346,0.0006702004,0.0009383972,0.00086883665,0.00074485724,0.0006967192],"category_scores_gemma":[0.0019044518,0.0003538143,0.0008259313,0.00042944297,0.0012750153,0.00042710366,0.00095166714,0.0007403875,0.00007025916],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025049844,0.00019160278,0.0155565385,0.000030719453,0.000083920146,0.00021441332,0.00015753001,0.97313267,0.00675762,0.0024380083,0.00015963061,0.0010269484],"study_design_scores_gemma":[0.00007113944,0.00006795265,0.0035536848,0.0000049012115,0.000011276576,0.000020251606,0.000047741036,0.99450994,0.001027289,0.0005879971,0.00008366031,0.000014067372],"about_ca_topic_score_codex":0.01614732,"about_ca_topic_score_gemma":0.006885062,"teacher_disagreement_score":0.01614732,"about_ca_system_score_codex":0.0011003504,"about_ca_system_score_gemma":0.00090014085,"threshold_uncertainty_score":0.032106638},"labels":[],"label_agreement":null},{"id":"W1859172354","doi":"10.1088/0004-637x/808/2/106","title":"MAPPING THE OUTER EDGE OF THE YOUNG STELLAR CLUSTER IN THE GALACTIC CENTER","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Stars; Astrophysics; Galactic Center; Astronomy; Supermassive black hole; Photometry (optics); Stellar density; Molecular cloud; Galaxy","score_opus":0.03156475783262535,"score_gpt":0.23838408342047815,"score_spread":0.2068193255878528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1859172354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991041,0.00009099408,0.00025936143,0.000005837274,0.0000015302339,0.0000034742523,0.00009363406,0.000019068179,0.00042203415],"genre_scores_gemma":[0.9982162,0.00006096678,0.0010866438,0.0000052658875,0.00000460592,0.0000032300554,0.0003602458,0.000008765174,0.000254068],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991524,0.000004617461,0.0000022894326,0.000029073555,0.000028396656,0.00002041071],"domain_scores_gemma":[0.99976736,0.000018847748,0.00006571726,0.000016382564,0.000053928918,0.00007787071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011351319,0.00015348363,0.00016462643,0.0009900876,0.00030406172,0.0003238833,0.00026190426,0.00015096735,0.00039021773],"category_scores_gemma":[0.000252012,0.00010254128,0.0001141988,0.00049442577,0.00014662242,0.00018004191,0.00036729424,0.00009673405,0.00022705852],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003978172,0.000056005825,0.8757291,0.000059091977,0.00006082599,0.00028592037,0.00090412144,0.0010799863,0.08844484,0.00021144804,0.0004366235,0.032334235],"study_design_scores_gemma":[0.000003090813,0.00004503847,0.9960997,0.0000045082406,0.000011979527,0.00009410576,0.00014183484,0.0008742117,0.0018790037,0.00004095531,0.00080150866,0.000004119675],"about_ca_topic_score_codex":0.010767778,"about_ca_topic_score_gemma":0.022803657,"teacher_disagreement_score":0.010767778,"about_ca_system_score_codex":0.00022866535,"about_ca_system_score_gemma":0.00014739297,"threshold_uncertainty_score":0.021410227},"labels":[],"label_agreement":null},{"id":"W1859339896","doi":"10.1088/0004-637x/806/2/206","title":"bicep2/<i>KECK ARRAY</i>. IV. OPTICAL CHARACTERIZATION AND PERFORMANCE OF THE bicep2 AND<i>KECK ARRAY</i>EXPERIMENTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"","keywords":"Cosmic microwave background; Cosmic background radiation; Microwave; Polarization (electrochemistry); Characterization (materials science); Inflation (cosmology); Cosmology","score_opus":0.017876078582014284,"score_gpt":0.23937742952366606,"score_spread":0.22150135094165177,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1859339896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7194933,0.0013612153,0.07629689,0.0012815623,0.0005184844,0.0018667759,0.029970294,0.0076773944,0.1615341],"genre_scores_gemma":[0.84656984,0.00033511518,0.110508665,0.00094595953,0.00012574348,0.0015469479,0.017642615,0.0013075859,0.021017557],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9987746,0.0001282837,0.000044327528,0.0003117275,0.00043150736,0.00030965605],"domain_scores_gemma":[0.9980525,0.00014815459,0.00033790086,0.0006285198,0.00058582425,0.0002471471],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018416177,0.00086155755,0.0004591203,0.0010141274,0.0011780569,0.0010221404,0.0010887225,0.0010787756,0.008241459],"category_scores_gemma":[0.0009101992,0.00058828853,0.0003908214,0.0010358888,0.00073666964,0.0012894338,0.0012362506,0.0010651331,0.0041011753],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0036073157,0.00049267616,0.026744522,0.0005127494,0.0003235744,0.0006377853,0.00039376708,0.00318102,0.8951456,0.010502724,0.023202486,0.035255793],"study_design_scores_gemma":[0.0002861542,0.0014979236,0.078515425,0.0000986957,0.00015620835,0.0011495148,0.00014501436,0.0066369628,0.78751653,0.0014381561,0.12238221,0.00017719965],"about_ca_topic_score_codex":0.0009134319,"about_ca_topic_score_gemma":0.0018705844,"teacher_disagreement_score":0.008241459,"about_ca_system_score_codex":0.0008870676,"about_ca_system_score_gemma":0.00069717946,"threshold_uncertainty_score":0.027570367},"labels":[],"label_agreement":null},{"id":"W1860272205","doi":"10.1088/0004-637x/732/1/46","title":"TRANSIENT EXTREMELY SOFT X-RAY EMISSION FROM THE UNUSUALLY BRIGHT CATACLYSMIC VARIABLE IN THE GLOBULAR CLUSTER M3: A NEW CV X-RAY LUMINOSITY RECORD?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Luminosity; Globular cluster; White dwarf; Cataclysmic variable star; Emission spectrum; Spectral index; Dwarf nova","score_opus":0.022740025878006002,"score_gpt":0.21797228187742732,"score_spread":0.19523225599942132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1860272205","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992094,0.0001296456,0.000089481444,0.000037755046,0.0000024306164,0.0000017944116,0.00013068461,0.000011164852,0.00038777888],"genre_scores_gemma":[0.99919695,0.00007632775,0.00019513367,0.000030389268,0.000011757981,0.0000024543215,0.00033946292,0.0000050407307,0.0001424942],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992764,0.0000042762126,0.000004267726,0.000028947892,0.00001567511,0.000019100664],"domain_scores_gemma":[0.9996736,0.000033923898,0.00014279662,0.00003470034,0.000027779393,0.00008728591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013846702,0.00014351377,0.00025707285,0.0004939307,0.00043274657,0.00070966064,0.00038175093,0.00035325417,0.00043539456],"category_scores_gemma":[0.00039603113,0.00014137737,0.00016795243,0.0007388491,0.00042006557,0.0002897064,0.0005654834,0.000350659,0.00012588082],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016786547,0.000038696562,0.96023333,0.000055065873,0.00003184113,0.0013000692,0.00079287076,0.000127518,0.028804742,0.00038759777,0.00038705036,0.0076733795],"study_design_scores_gemma":[0.000003447554,0.000032252097,0.9968893,0.0000062754184,0.000010343466,0.0009817099,0.00015350062,0.00019349597,0.0006593545,0.000104047125,0.00095975504,0.0000065257323],"about_ca_topic_score_codex":0.0048123663,"about_ca_topic_score_gemma":0.010570195,"teacher_disagreement_score":0.0048123663,"about_ca_system_score_codex":0.00045446446,"about_ca_system_score_gemma":0.00017282384,"threshold_uncertainty_score":0.009568691},"labels":[],"label_agreement":null},{"id":"W1860808629","doi":"10.1088/0004-637x/806/1/112","title":"THE Q/U IMAGING EXPERIMENT: POLARIZATION MEASUREMENTS OF RADIO SOURCES AT 43 AND 95 GHz","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Polarization (electrochemistry); CMB cold spot; Cosmic microwave background; Planck; Linear polarization; Radio telescope; Stokes parameters; Amplitude; Telescope","score_opus":0.015250195387454204,"score_gpt":0.22310369787955805,"score_spread":0.20785350249210385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1860808629","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9881902,0.0002841446,0.0030628613,0.0001240098,0.000022654509,0.000032102213,0.0041938294,0.0002554694,0.0038348017],"genre_scores_gemma":[0.9849925,0.00016495438,0.0059750355,0.00012893435,0.000095634576,0.000047470225,0.007862082,0.00007099845,0.00066233304],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99951196,0.000074082,0.000024062196,0.00012243705,0.0001362374,0.00013127776],"domain_scores_gemma":[0.9989398,0.0001104091,0.0004337239,0.00017835897,0.00011207745,0.00022570115],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089450437,0.00026730716,0.0002014833,0.0017417321,0.00035466603,0.00063174596,0.00039366266,0.00028465225,0.0011549554],"category_scores_gemma":[0.0010242884,0.00026181136,0.00030070893,0.0013577143,0.00027138507,0.00040869656,0.00068784493,0.00039565135,0.00035284285],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091030414,0.00029663142,0.89213777,0.000111348134,0.00030091358,0.0004604384,0.0006263132,0.0016796719,0.050574474,0.0016142905,0.008795327,0.0424926],"study_design_scores_gemma":[0.00005418038,0.00007778237,0.98806506,0.000009607247,0.000051787163,0.0002967511,0.00006568925,0.0014896978,0.004840295,0.00020529273,0.0048218085,0.000022091452],"about_ca_topic_score_codex":0.002716499,"about_ca_topic_score_gemma":0.0045864517,"teacher_disagreement_score":0.002716499,"about_ca_system_score_codex":0.0002128776,"about_ca_system_score_gemma":0.00018000447,"threshold_uncertainty_score":0.0054013133},"labels":[],"label_agreement":null},{"id":"W1861812582","doi":"10.1088/0004-637x/704/2/l80","title":"DIVERSE KINEMATIC SIGNATURES FROM REVERBERATION MAPPING OF THE BROAD-LINE REGION IN AGNs","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":179,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Reverberation mapping; Physics; Astrophysics; Active galactic nucleus; Observatory; Reverberation; Astronomy; Line (geometry); Luminosity; Kinematics; Emission spectrum; Spectral line; Galaxy; Geometry; Acoustics","score_opus":0.015191819242397422,"score_gpt":0.22851188958314594,"score_spread":0.2133200703407485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1861812582","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974692,0.00015448571,0.0008548578,0.000013780432,0.000004697512,0.0000051441098,0.00037849415,0.0000475203,0.0010718853],"genre_scores_gemma":[0.9975268,0.00012843467,0.00068552984,0.000014259034,0.000015060959,0.0000062774257,0.0010705328,0.00002171305,0.0005313748],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998863,0.0000151361555,0.0000064366886,0.000028444401,0.000034316323,0.000029409297],"domain_scores_gemma":[0.99961853,0.00007351362,0.00013625727,0.00004669656,0.00005625111,0.00006873062],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025898658,0.0002204497,0.0002327847,0.0012973548,0.00017552,0.0003868883,0.00021097316,0.00019969675,0.0011442471],"category_scores_gemma":[0.00076912215,0.00016285111,0.00022769978,0.00073714403,0.00017971895,0.00018076782,0.00039991032,0.00020423195,0.00048071562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011717246,0.000093445604,0.6692488,0.000083136736,0.00013042065,0.0012401256,0.0014215962,0.0009370454,0.2723468,0.0001947102,0.00037421435,0.052757904],"study_design_scores_gemma":[0.0000030146757,0.000046492725,0.9970487,0.0000029681044,0.000013561494,0.0005767115,0.00007243637,0.00017716197,0.0016996823,0.000027956874,0.0003266217,0.000004705007],"about_ca_topic_score_codex":0.0014047272,"about_ca_topic_score_gemma":0.0024694907,"teacher_disagreement_score":0.0014047272,"about_ca_system_score_codex":0.00009444541,"about_ca_system_score_gemma":0.00006435273,"threshold_uncertainty_score":0.0038279295},"labels":[],"label_agreement":null},{"id":"W1861925557","doi":"10.1088/0004-637x/807/1/83","title":"CONFIRMATION OF HOSTLESS TYPE Ia SUPERNOVAE USING<i>HUBBLE SPACE TELESCOPE</i>IMAGING","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Astronomy; Globular cluster; Galaxy; Supernova; Dwarf galaxy; Luminosity; Elliptical galaxy; Hubble space telescope; Redshift; Population; Galaxy cluster","score_opus":0.026042539193708768,"score_gpt":0.2711841487160641,"score_spread":0.24514160952235534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1861925557","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931391,0.00044638326,0.0015109141,0.00006998822,0.00002202336,0.000020809619,0.0009188805,0.00011527624,0.0037566484],"genre_scores_gemma":[0.99626994,0.00013031434,0.0018676176,0.00007037451,0.00001939837,0.000006678029,0.0010831488,0.00001102515,0.00054155244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997774,0.0000191518,0.00002865628,0.00006123428,0.00004552863,0.000068131434],"domain_scores_gemma":[0.99890876,0.00009896492,0.0003407805,0.00010195793,0.00019316502,0.0003563813],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048668133,0.00042828787,0.0002738219,0.0015244561,0.00053268805,0.0007366394,0.00057711924,0.00047151762,0.0019247404],"category_scores_gemma":[0.0008238692,0.00019258946,0.0003948806,0.0005760715,0.00041818552,0.00033640827,0.00052327715,0.00033875604,0.0004336867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023014103,0.00005824445,0.90440446,0.00007931011,0.00008707838,0.0019084023,0.00020480025,0.00032978633,0.08551081,0.0003568809,0.0006424417,0.006187656],"study_design_scores_gemma":[0.000011618614,0.00010561485,0.9819157,0.00002216038,0.000044930508,0.0027365596,0.00018427675,0.00087808527,0.012058617,0.00018164658,0.0018493193,0.000011521559],"about_ca_topic_score_codex":0.006911041,"about_ca_topic_score_gemma":0.014804952,"teacher_disagreement_score":0.006911041,"about_ca_system_score_codex":0.00038622908,"about_ca_system_score_gemma":0.00024154695,"threshold_uncertainty_score":0.013741612},"labels":[],"label_agreement":null},{"id":"W1862641251","doi":"10.1088/0004-637x/812/2/95","title":"LONG-TERM TIMING AND EMISSION BEHAVIOR OF THE YOUNG CRAB-LIKE PULSAR PSR B0540–69","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Goddard Space Flight Center; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Pulsar; Glitch; Physics; Astrophysics; Crab Pulsar; Neutron star; Noise (video); Population; Static timing analysis; Astronomy","score_opus":0.027302804489921458,"score_gpt":0.33586745781103555,"score_spread":0.3085646533211141,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1862641251","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99901915,0.000049026847,0.00017717281,0.000017372286,0.000002371194,0.0000019155832,0.00039483563,0.000020343428,0.0003178238],"genre_scores_gemma":[0.9978321,0.00003607011,0.00031709397,0.00000822262,0.0000062914255,0.0000039850515,0.0016893133,0.000010103034,0.00009676457],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988234,0.00001229152,0.000008737506,0.00003738247,0.000026240392,0.000033056334],"domain_scores_gemma":[0.99942315,0.00008629165,0.0002453396,0.000038571405,0.00008606096,0.00012073497],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000294464,0.00023799148,0.00025137988,0.0011237122,0.00034145208,0.00033917098,0.00024697607,0.00030027807,0.0004709566],"category_scores_gemma":[0.001116245,0.00017652888,0.00022801198,0.00095425337,0.00021759338,0.00021916354,0.00034977173,0.00030091917,0.00013700068],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006311543,0.00023656171,0.8124725,0.00013706557,0.0003993654,0.001208429,0.00086334575,0.034178827,0.110282086,0.0013617146,0.002097113,0.036131904],"study_design_scores_gemma":[0.000014410233,0.00009119734,0.9813887,0.000012054413,0.000038026606,0.00019565546,0.000073938,0.015785532,0.0014533938,0.00013435961,0.00078896765,0.000023869308],"about_ca_topic_score_codex":0.01233251,"about_ca_topic_score_gemma":0.01925274,"teacher_disagreement_score":0.01233251,"about_ca_system_score_codex":0.00032335878,"about_ca_system_score_gemma":0.00022757609,"threshold_uncertainty_score":0.02452141},"labels":[],"label_agreement":null},{"id":"W1864790716","doi":"10.1088/0004-637x/806/1/101","title":"LoCuSS: THE SLOW QUENCHING OF STAR FORMATION IN CLUSTER GALAXIES AND THE NEED FOR PRE-PROCESSING","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":253,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Science and Technology Facilities Council; National Science Foundation","keywords":"Velocity dispersion; Galaxy; Star formation; Galaxy cluster; Cluster (spacecraft); Brightest cluster galaxy; Elliptical galaxy; Luminous infrared galaxy; Peculiar galaxy","score_opus":0.010411295675167326,"score_gpt":0.2304401209816663,"score_spread":0.22002882530649898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1864790716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985421,0.00009316332,0.0008897687,0.000018125982,7.9862014e-7,0.000005153519,0.000050819624,0.00002948415,0.00037058888],"genre_scores_gemma":[0.99878496,0.00003447513,0.0008361343,0.00001124544,0.000002719998,0.00000396707,0.00011305157,0.000010512285,0.00020293548],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997631,0.00003785397,0.000012284206,0.000075373566,0.00006808908,0.000043409065],"domain_scores_gemma":[0.9987477,0.0003279511,0.0003704192,0.00022571973,0.00014003915,0.000188152],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050047203,0.00018480359,0.0002429626,0.00048450558,0.0003289171,0.0007653926,0.0004107859,0.00023763232,0.0007072648],"category_scores_gemma":[0.0025555997,0.00018125039,0.0001737415,0.00042984026,0.00051650754,0.00074202573,0.0005552277,0.00023954612,0.0002475709],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039667144,0.00003950592,0.89400214,0.00004453239,0.00006744073,0.00026364156,0.00090157805,0.0026627667,0.06279566,0.00057772844,0.00014191613,0.038106292],"study_design_scores_gemma":[0.000005225347,0.00012563758,0.9888437,0.0000038062624,0.000013192439,0.0003249837,0.00021552155,0.0028556038,0.0066752,0.0004391906,0.00049009995,0.000007875101],"about_ca_topic_score_codex":0.0029943404,"about_ca_topic_score_gemma":0.0031636218,"teacher_disagreement_score":0.0029943404,"about_ca_system_score_codex":0.00039662432,"about_ca_system_score_gemma":0.00019268774,"threshold_uncertainty_score":0.0059537888},"labels":[],"label_agreement":null},{"id":"W1871368792","doi":"10.1088/0004-637x/700/1/331","title":"CfA3: 185 TYPE Ia SUPERNOVA LIGHT CURVES FROM THE CfA","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":518,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; University of Waterloo","funders":"","keywords":"Physics; Photometry (optics); Light curve; Astrophysics; Supernova; Astronomy; Galaxy; Stars; Cosmology","score_opus":0.011136331470138105,"score_gpt":0.2411736441644659,"score_spread":0.2300373126943278,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1871368792","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9445033,0.00022455331,0.0017758404,0.00005832827,0.0000208629,0.000052182902,0.048268944,0.00058279483,0.0045132],"genre_scores_gemma":[0.8899831,0.00007983738,0.0035963673,0.000074262345,0.000027201197,0.000041581116,0.1050209,0.00016985873,0.001006926],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99953115,0.00003536965,0.000043835003,0.00009410684,0.00017745662,0.000118073345],"domain_scores_gemma":[0.99722135,0.00018779332,0.0005854475,0.00054540177,0.00080054614,0.00065948005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010087576,0.00055544474,0.000403246,0.0036527799,0.000554416,0.0007670987,0.00049624284,0.00037832005,0.0028148459],"category_scores_gemma":[0.0017333439,0.00022038077,0.0008563628,0.003145894,0.00017790026,0.00032397316,0.00051986077,0.00038254124,0.0020036888],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007903895,0.00019630307,0.9297496,0.00008209917,0.00023755051,0.00024983365,0.00025393668,0.001829089,0.014916265,0.0003145797,0.02019878,0.031181622],"study_design_scores_gemma":[0.000010086248,0.000042102976,0.99360776,0.0000054132047,0.000011687963,0.0002261189,0.000026826676,0.0007436311,0.00088624837,0.00005608767,0.004373077,0.000011084192],"about_ca_topic_score_codex":0.03324323,"about_ca_topic_score_gemma":0.052389093,"teacher_disagreement_score":0.03324323,"about_ca_system_score_codex":0.00092250755,"about_ca_system_score_gemma":0.00050292,"threshold_uncertainty_score":0.066099465},"labels":[],"label_agreement":null},{"id":"W1873146751","doi":"10.1088/0004-637x/806/1/129","title":"SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. II.<i>SWIFT</i>AND<i>HST</i>REVERBERATION MAPPING OF THE ACCRETION DISK OF NGC 5548","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":308,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Natural Sciences and Engineering Research Council of Canada; University of California, Santa Barbara; Jet Propulsion Laboratory; Space Telescope Science Institute; American Academy in Rome; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Georgia State University; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Science and Technology Facilities Council; National Research Foundation; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; California Institute of Technology; Ohio State University; Danmarks Frie Forskningsfond; National Science Foundation","keywords":"Reverberation mapping; Gravitational microlensing; Quasar; Balmer series; Galaxy; Active galactic nucleus; Accretion (finance); Light curve","score_opus":0.023394444716234426,"score_gpt":0.23748087937330342,"score_spread":0.214086434657069,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1873146751","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7621438,0.0012194181,0.01282522,0.0018214881,0.0003965962,0.001559786,0.16449454,0.0020693664,0.053469796],"genre_scores_gemma":[0.52829427,0.0005457618,0.042692363,0.0009013086,0.00027730045,0.00091735413,0.38823807,0.0003508533,0.037782725],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99957997,0.000059883198,0.000019218101,0.00008849707,0.0001387017,0.00011371986],"domain_scores_gemma":[0.9985025,0.000076658645,0.00024983482,0.000214645,0.00039788004,0.0005584494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012713489,0.0006831709,0.00030754393,0.0018188288,0.00046080814,0.0006418117,0.0005787362,0.00031295366,0.0035363955],"category_scores_gemma":[0.0007660989,0.00023258058,0.0002262203,0.0007575932,0.00022762992,0.00040092933,0.0009030952,0.00043619532,0.003363494],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024443525,0.0010571658,0.51875836,0.00026392925,0.00028991795,0.0016127733,0.0016058432,0.0016431598,0.0732656,0.002045322,0.08800025,0.3090133],"study_design_scores_gemma":[0.00020015053,0.00042714868,0.9184331,0.000022191129,0.000052146403,0.00043115253,0.00021707744,0.001567307,0.006034425,0.00025708025,0.072343074,0.000015186152],"about_ca_topic_score_codex":0.020063758,"about_ca_topic_score_gemma":0.026104419,"teacher_disagreement_score":0.020063758,"about_ca_system_score_codex":0.00056773896,"about_ca_system_score_gemma":0.0009349853,"threshold_uncertainty_score":0.039893925},"labels":[],"label_agreement":null},{"id":"W1877425211","doi":"10.1088/0004-637x/815/2/97","title":"LOW ANGULAR MOMENTUM IN CLUMPY, TURBULENT DISK GALAXIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência, Tecnologia e Inovação; Swinburne University of Technology; National Aeronautics and Space Administration; California Institute of Technology; U.S. Department of State; Space Telescope Science Institute; National Science Foundation","keywords":"Angular momentum; Bulge; Galaxy; Spiral galaxy; Specific relative angular momentum; Stellar mass; Star formation; Low Mass; Galaxy formation and evolution; Stars","score_opus":0.009066566160726753,"score_gpt":0.21463544346650854,"score_spread":0.20556887730578177,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1877425211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997782,0.000023624876,0.00006400075,0.0000015442465,3.258573e-7,8.612347e-7,0.000021037702,0.000004723606,0.00010557253],"genre_scores_gemma":[0.9998122,0.000009910918,0.0000707879,0.0000018683952,9.702948e-7,7.869535e-7,0.000059515667,0.0000012749832,0.000042793876],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999845,0.000015256626,0.000012114049,0.000051513412,0.00003255054,0.000043508073],"domain_scores_gemma":[0.99904555,0.000115003895,0.00043089807,0.000075529,0.00007579107,0.00025726174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025058494,0.00029021426,0.00026052378,0.001860612,0.00035303042,0.00082646037,0.0003075589,0.0002814654,0.00044287046],"category_scores_gemma":[0.0010239044,0.0001819376,0.0001107374,0.0009079367,0.00062964787,0.00037950464,0.0006819223,0.0001525452,0.0001417144],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025383814,0.000034620185,0.96747375,0.00001637989,0.000034996687,0.00017515241,0.0005961415,0.00040238787,0.027690807,0.00016559297,0.00003197733,0.003124416],"study_design_scores_gemma":[0.00000469961,0.00004615619,0.9972907,0.0000015939437,0.000009218904,0.00012587507,0.00016572796,0.0005041213,0.0017118593,0.00006582007,0.000070892354,0.0000033973758],"about_ca_topic_score_codex":0.002746671,"about_ca_topic_score_gemma":0.0028781607,"teacher_disagreement_score":0.002746671,"about_ca_system_score_codex":0.00042376234,"about_ca_system_score_gemma":0.00008952613,"threshold_uncertainty_score":0.005461335},"labels":[],"label_agreement":null},{"id":"W1885625861","doi":"10.1086/338479","title":"Halo Substructure and Disk Heating in a Λ Cold Dark Matter Universe","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; Pacific Institute for the Mathematical Sciences; University of Victoria","funders":"","keywords":"Substructure; Cold dark matter; Milky Way; Halo; Dark matter; Universe; Hot dark matter; Galactic halo","score_opus":0.0071282363472757425,"score_gpt":0.2400807172869393,"score_spread":0.23295248093966356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1885625861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99919814,0.000055144126,0.00020326894,0.000035550725,9.362671e-7,8.3191003e-7,0.00001302476,0.000008065452,0.0004850319],"genre_scores_gemma":[0.9996706,0.000043964716,0.00007933016,0.000009962018,0.0000019970034,7.193711e-7,0.000012036009,0.0000035789126,0.00017766259],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999615,0.000010989377,0.0000010624826,0.0000061072533,0.000004255653,0.000016073662],"domain_scores_gemma":[0.99950683,0.0001790393,0.00012528076,0.000050712562,0.000022973067,0.000115156115],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022387331,0.00023421175,0.00018033948,0.0003042334,0.00046233312,0.00070511794,0.00031121488,0.0002789281,0.001130015],"category_scores_gemma":[0.0013881259,0.00021220764,0.0002342859,0.00023582511,0.000614539,0.0005843934,0.000800439,0.00027971025,0.0001246139],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010176226,0.00018645158,0.4886281,0.000087765016,0.00029752683,0.0014547289,0.0016350545,0.4464309,0.027491909,0.021557804,0.0008683311,0.010343861],"study_design_scores_gemma":[0.00023267585,0.00025730956,0.41987216,0.000023114679,0.00020431285,0.000397258,0.00075363036,0.55299795,0.0041729454,0.01981249,0.0012169423,0.0000592101],"about_ca_topic_score_codex":0.0107615935,"about_ca_topic_score_gemma":0.0069859335,"teacher_disagreement_score":0.0107615935,"about_ca_system_score_codex":0.00071867637,"about_ca_system_score_gemma":0.00017109401,"threshold_uncertainty_score":0.021397889},"labels":[],"label_agreement":null},{"id":"W1887246147","doi":"10.1088/0004-637x/811/2/153","title":"PROBING THE IONIZATION STATES OF POLYCYCLIC AROMATIC HYDROCARBONS VIA THE 15–20<i>μ</i>m EMISSION BANDS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Galaxy; Ionization; Reflection nebula; Spectral bands; Cirrus; Molecular cloud; Spatial distribution; Point source","score_opus":0.011490412844099972,"score_gpt":0.23250657350297946,"score_spread":0.2210161606588795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1887246147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992347,0.00003784313,0.00014022265,0.00000537936,4.566664e-7,0.0000012339439,0.0002080398,0.000008348959,0.00036375894],"genre_scores_gemma":[0.99877304,0.00003630445,0.0004090981,0.0000069046887,0.0000022379909,0.0000022716738,0.00064808334,0.000002685981,0.000119281234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999918,0.000008931765,0.000004679756,0.00002576489,0.000019650099,0.00002297428],"domain_scores_gemma":[0.999371,0.00010043276,0.00034313704,0.00004392439,0.000060847386,0.00008070338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001410768,0.00016701278,0.00010264597,0.00084617216,0.00014358659,0.00025099597,0.00013947001,0.00012545122,0.0013839666],"category_scores_gemma":[0.0004243677,0.000119003154,0.00013186784,0.0006913122,0.00015499626,0.00014014884,0.00024697464,0.000118594326,0.00029229853],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057257625,0.000017465305,0.9733724,0.00001029512,0.000038018185,0.00003753235,0.00006005512,0.00018269851,0.021793092,0.000038139548,0.00007077106,0.0043221586],"study_design_scores_gemma":[8.254634e-7,0.0000127750645,0.99843687,8.2480483e-7,0.000007367393,0.000048965758,0.000028408587,0.00015895089,0.0011909164,0.00001713436,0.000095167336,0.0000016889504],"about_ca_topic_score_codex":0.002705663,"about_ca_topic_score_gemma":0.007040009,"teacher_disagreement_score":0.002705663,"about_ca_system_score_codex":0.000115193405,"about_ca_system_score_gemma":0.00008029003,"threshold_uncertainty_score":0.005379796},"labels":[],"label_agreement":null},{"id":"W1894385335","doi":"10.3847/0004-637x/819/1/35","title":"RAPIDLY RISING TRANSIENTS IN THE SUPERNOVA—SUPERLUMINOUS SUPERNOVA GAP","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":153,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Defence Research and Development Canada; University of Toronto","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Science and Technology Facilities Council; Israel Science Foundation; Planning and Budgeting Committee of the Council for Higher Education of Israel; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; York University; Ohio State University; National Research Foundation; Carnegie Mellon University; Office of Science; University of Washington; Alfred P. Sloan Foundation; Princeton University; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Jet Propulsion Laboratory; California Institute of Technology; U.S. Department of Energy; W. M. Keck Foundation; National Science Foundation","keywords":"Supernova; Physics; Astrophysics; Magnetar; Light curve; Gamma-ray burst; White dwarf; Astronomy; Spectral line; Stars; Neutron star","score_opus":0.017378860585404766,"score_gpt":0.23895452435094677,"score_spread":0.221575663765542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1894385335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99739766,0.00022733405,0.0006744225,0.00002316186,0.000009448172,0.000008147686,0.000112449045,0.00006311436,0.0014843],"genre_scores_gemma":[0.9993957,0.00004230654,0.00027626532,0.000016648524,0.000007124598,0.0000028889192,0.00013735073,0.000005237102,0.00011640075],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999361,0.0000067494548,0.000004627702,0.000019385492,0.000015453605,0.000017602246],"domain_scores_gemma":[0.999521,0.000077285324,0.00018816431,0.00006046101,0.00003310788,0.0001199577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002140677,0.00021559966,0.0002673013,0.00067034987,0.00033701173,0.00055760366,0.00031012256,0.00036348178,0.0010056414],"category_scores_gemma":[0.00041132077,0.00013498041,0.00025471143,0.00039180435,0.00025273193,0.000226675,0.0005086183,0.00034705436,0.00022030997],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011183636,0.00024176518,0.7077723,0.00012321526,0.00018424196,0.011249846,0.00052724296,0.0021092594,0.24255966,0.0027575598,0.0009702404,0.03038631],"study_design_scores_gemma":[0.00002377111,0.00034942885,0.97480065,0.000019118303,0.000038130147,0.007469355,0.00013278885,0.002017559,0.011301512,0.00082259066,0.0030053197,0.000019757637],"about_ca_topic_score_codex":0.0008087919,"about_ca_topic_score_gemma":0.0010584379,"teacher_disagreement_score":0.0010056414,"about_ca_system_score_codex":0.00026785975,"about_ca_system_score_gemma":0.00007811416,"threshold_uncertainty_score":0.0033642054},"labels":[],"label_agreement":null},{"id":"W1894915454","doi":"10.1086/379800","title":"The Pulsar/White Dwarf/Planet System in M4: Improved Astrometry","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"White dwarf; Proper motion; Globular cluster; Millisecond pulsar; Astrometry; Pulsar; Brown dwarf; Star cluster; Circumbinary planet","score_opus":0.006793883508529723,"score_gpt":0.20779224632613064,"score_spread":0.20099836281760092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1894915454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99653983,0.00008733585,0.0008528364,0.00007155812,0.0000071442773,0.0000100455145,0.0006224193,0.000101004,0.0017079541],"genre_scores_gemma":[0.98861456,0.00007327725,0.0068225414,0.0000254208,0.000021779675,0.000012496988,0.0021262849,0.000028602863,0.0022749866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998258,0.000031229236,0.000014865559,0.0000369314,0.000053956144,0.00003724684],"domain_scores_gemma":[0.99958545,0.000040066563,0.00010075173,0.000085471824,0.000110005145,0.000078224344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047399278,0.00022093747,0.00025964994,0.001695612,0.00043140835,0.000440751,0.0005338872,0.0002942106,0.0026551925],"category_scores_gemma":[0.0008595924,0.000106195796,0.00019151255,0.0008632553,0.00021416346,0.00045352473,0.0008084009,0.00026600293,0.0010552699],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049165956,0.000114354334,0.91252494,0.000061931925,0.0000383012,0.00049081305,0.0005135657,0.0011184801,0.045095272,0.0004992918,0.0013292969,0.037722073],"study_design_scores_gemma":[0.00002028692,0.00018017639,0.98317564,0.000008886482,0.00003442592,0.0006271319,0.00014781016,0.0022205648,0.0073163738,0.00029575697,0.0059609776,0.000011953188],"about_ca_topic_score_codex":0.006970093,"about_ca_topic_score_gemma":0.009361668,"teacher_disagreement_score":0.006970093,"about_ca_system_score_codex":0.0004546868,"about_ca_system_score_gemma":0.00032187137,"threshold_uncertainty_score":0.013859093},"labels":[],"label_agreement":null},{"id":"W1895121002","doi":"10.1088/0004-637x/811/1/18","title":"<i>β</i>PICTORIS’ INNER DISK IN POLARIZED LIGHT AND NEW ORBITAL PARAMETERS FOR<i>β</i>PICTORIS<i>b</i>","year":2015,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Debris disk; Position angle; Astrophysics; RADIUS; Orbital inclination; Planet; Orbital eccentricity; Eccentricity (behavior); Exoplanet; Scale height; Thick disk; Planetary system; Halo; Binary number; Galaxy","score_opus":0.021472508828213634,"score_gpt":0.22929519347855634,"score_spread":0.2078226846503427,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1895121002","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9584378,0.00068392366,0.012777219,0.0003502691,0.00013111437,0.00003683439,0.0019531206,0.00066917867,0.024960507],"genre_scores_gemma":[0.9915215,0.00019387604,0.0057738926,0.000114367016,0.000032419877,0.000028316488,0.0017296331,0.00010965943,0.0004963884],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992454,0.000008013409,0.0000037062339,0.000034460823,0.000014770547,0.000014546863],"domain_scores_gemma":[0.99975985,0.00003428588,0.0000776595,0.00004924405,0.000035506186,0.000043361342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019647786,0.00040212262,0.00017225591,0.00087786384,0.0004315566,0.0009682365,0.00031578474,0.00043214613,0.0016443736],"category_scores_gemma":[0.000467139,0.00030604258,0.0002713103,0.0005956707,0.00029070274,0.0005338009,0.0003073206,0.0007130825,0.00068623875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010713546,0.00023144273,0.7023112,0.00034896584,0.00024577344,0.0025504765,0.00092276605,0.016739555,0.1397522,0.0071093775,0.025555914,0.103160985],"study_design_scores_gemma":[0.000060502003,0.000074773656,0.924306,0.000073867,0.000120774755,0.0016150656,0.00027426734,0.026520247,0.014617029,0.002053352,0.03021847,0.0000657418],"about_ca_topic_score_codex":0.0025485863,"about_ca_topic_score_gemma":0.0029562984,"teacher_disagreement_score":0.0025485863,"about_ca_system_score_codex":0.00043104618,"about_ca_system_score_gemma":0.00015315252,"threshold_uncertainty_score":0.0055009723},"labels":[],"label_agreement":null},{"id":"W1895670736","doi":"10.1088/0004-637x/696/1/853","title":"Lyα RADIATIVE TRANSFER IN COSMOLOGICAL SIMULATIONS USING ADAPTIVE MESH REFINEMENT","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Redshift; Astrophysics; Galaxy; Surface brightness; Radiative transfer; Emissivity; Adaptive mesh refinement; Halo; Field (mathematics); Brightness; Interstellar medium; Intergalactic travel; Astronomy; Optics","score_opus":0.0210226886133734,"score_gpt":0.24826698499352515,"score_spread":0.22724429638015176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1895670736","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.23801059,0.00035166065,0.73824656,0.0006870974,0.00020317921,0.0003139527,0.00067281944,0.0032779023,0.018236233],"genre_scores_gemma":[0.6376804,0.00020180618,0.35578394,0.00018804752,0.000066694614,0.0007445031,0.0006105432,0.0007838371,0.003940219],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99971014,0.00013695999,0.000015885766,0.000026867596,0.00007639945,0.000033732216],"domain_scores_gemma":[0.9986386,0.0008122431,0.00012175765,0.00011821297,0.00019638072,0.00011273324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00094431755,0.0006256269,0.0006575722,0.00059147354,0.0006984923,0.0007047867,0.0019023636,0.0013460104,0.002540125],"category_scores_gemma":[0.0042873854,0.00042424657,0.0006849575,0.0006101816,0.0007464113,0.00060801744,0.0012998526,0.00089835015,0.00050523836],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000044868117,0.00003642141,0.0011489654,0.000026442693,0.000020941843,0.000058553665,0.000059175552,0.98735154,0.0014388185,0.0047859894,0.00047460236,0.004553643],"study_design_scores_gemma":[0.000016317399,0.000005775266,0.00006723232,0.0000021797964,0.0000012189861,0.0000040311897,0.000005024356,0.9987369,0.00015037777,0.0007155916,0.00029239504,0.000002884249],"about_ca_topic_score_codex":0.0142682195,"about_ca_topic_score_gemma":0.008258856,"teacher_disagreement_score":0.0142682195,"about_ca_system_score_codex":0.0010630571,"about_ca_system_score_gemma":0.0011276654,"threshold_uncertainty_score":0.02837032},"labels":[],"label_agreement":null},{"id":"W1896473331","doi":"10.1088/0004-637x/791/1/71","title":"ACCELERATION OF RELATIVISTIC ELECTRONS BY MAGNETOHYDRODYNAMIC TURBULENCE: IMPLICATIONS FOR NON-THERMAL EMISSION FROM BLACK HOLE ACCRETION DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Magnetohydrodynamics; Fermi acceleration; Magnetohydrodynamic drive; Particle acceleration; Accretion (finance); Acceleration; Magnetohydrodynamic turbulence; Turbulence; Electron","score_opus":0.009076548136674254,"score_gpt":0.2425543571501261,"score_spread":0.23347780901345186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1896473331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9855575,0.00016868979,0.011485317,0.00022406282,0.000013288044,0.000015521377,0.0000331195,0.00007517872,0.002427292],"genre_scores_gemma":[0.9990029,0.00003746335,0.00080266956,0.000010852633,0.000005309467,0.000003692225,0.000008878617,0.000007669439,0.000120506054],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991715,0.000030105468,0.000006264279,0.0000085824795,0.000017258282,0.000020504609],"domain_scores_gemma":[0.9992281,0.00037931043,0.0001952036,0.000061993196,0.000044671193,0.00009069002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036617563,0.00055713055,0.00034982892,0.00031091063,0.00046077828,0.00068999117,0.0005471639,0.0004004679,0.00057496945],"category_scores_gemma":[0.0021095884,0.00018442319,0.00035600597,0.00023501682,0.00077076786,0.00062452623,0.0007663676,0.00034029208,0.00007657514],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043440447,0.00015783084,0.041435562,0.00011605099,0.000066331784,0.0014559515,0.00035354964,0.8622864,0.04848485,0.038799793,0.00037172495,0.0060375077],"study_design_scores_gemma":[0.00005471845,0.000057175435,0.0057222894,0.000004284638,0.000009144065,0.000071329974,0.000031564676,0.98600185,0.0033799862,0.004549603,0.0001031219,0.000014923925],"about_ca_topic_score_codex":0.0026239417,"about_ca_topic_score_gemma":0.0011111298,"teacher_disagreement_score":0.0026239417,"about_ca_system_score_codex":0.0005655564,"about_ca_system_score_gemma":0.00021673077,"threshold_uncertainty_score":0.0052173138},"labels":[],"label_agreement":null},{"id":"W1900031469","doi":"10.1088/0004-637x/810/1/51","title":"DIRECT FORMATION OF SUPERMASSIVE BLACK HOLES IN METAL-ENRICHED GAS AT THE HEART OF HIGH-REDSHIFT GALAXY MERGERS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Supermassive black hole; Galaxy merger; Galaxy; Angular momentum; Gravitational collapse; Black hole (networking); Spin-flip; Gravitational wave; Star formation","score_opus":0.011898353800281761,"score_gpt":0.22063047045525952,"score_spread":0.20873211665497776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1900031469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940859,0.00006198869,0.0019390915,0.00027501088,0.000021357708,0.000018103057,0.00014275285,0.00007242046,0.0033833256],"genre_scores_gemma":[0.998355,0.000032168868,0.0010098424,0.000068114154,0.000012287616,0.000011148903,0.00011102075,0.000018519117,0.00038192366],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999027,0.000024787589,0.0000035787332,0.00001473175,0.000015422142,0.000038786093],"domain_scores_gemma":[0.99955314,0.00014246508,0.00007750835,0.000028537723,0.000033331922,0.0001650197],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028071768,0.0005572493,0.00049222953,0.00032473632,0.000618696,0.0011653034,0.0010341356,0.0012326051,0.0011849491],"category_scores_gemma":[0.0014766017,0.00031532175,0.0006286501,0.00021698489,0.0010758159,0.0006294273,0.0009088342,0.00069783756,0.00013743035],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034812122,0.00022112763,0.039114818,0.00003712103,0.0001207848,0.0007190128,0.0002360793,0.94647723,0.005151126,0.005078651,0.0007912136,0.0017047045],"study_design_scores_gemma":[0.00010129204,0.00006442174,0.0070109507,0.0000061835462,0.000019771463,0.000042420477,0.00009666663,0.99070835,0.0005383765,0.0011796324,0.00022109914,0.000010798467],"about_ca_topic_score_codex":0.018366005,"about_ca_topic_score_gemma":0.010675173,"teacher_disagreement_score":0.018366005,"about_ca_system_score_codex":0.0008965104,"about_ca_system_score_gemma":0.0006482911,"threshold_uncertainty_score":0.036518216},"labels":[],"label_agreement":null},{"id":"W1905014688","doi":"10.1088/0004-637x/794/2/141","title":"GRAVITATIONAL WAVES FROM INDIVIDUAL SUPERMASSIVE BLACK HOLE BINARIES IN CIRCULAR ORBITS: LIMITS FROM THE NORTH AMERICAN NANOHERTZ OBSERVATORY FOR GRAVITATIONAL WAVES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Physics; Gravitational wave; Pulsar; Astrophysics; Supermassive black hole; Observatory; Gravitational-wave observatory; Astronomy; Black hole (networking); LIGO; Sky; Binary black hole; Galaxy","score_opus":0.02151914176255585,"score_gpt":0.2860900087847256,"score_spread":0.26457086702216975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1905014688","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99426407,0.00024940073,0.0036958791,0.00013470105,0.000004559625,0.000008847092,0.00044286644,0.00003725692,0.0011624206],"genre_scores_gemma":[0.99548423,0.000111348985,0.003050923,0.0000299564,0.000016030117,0.00001040964,0.001115398,0.000011980029,0.0001698104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99957174,0.0000800941,0.000029802772,0.000105397135,0.00016082611,0.000052088555],"domain_scores_gemma":[0.99436873,0.0024393648,0.0016493768,0.00070573285,0.00038189138,0.00045490635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014507925,0.00024295726,0.00032491225,0.0018700848,0.0006618905,0.0008323986,0.00055720756,0.00030144348,0.00082669547],"category_scores_gemma":[0.0056000566,0.00027741666,0.0003066904,0.0011563253,0.0005059984,0.0007718315,0.0013497324,0.00042227918,0.00016739254],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027375246,0.000088383844,0.93484885,0.00006261104,0.00019120116,0.00021799613,0.0005888352,0.01047273,0.010462319,0.0031925493,0.000841227,0.038759463],"study_design_scores_gemma":[0.000031755422,0.00007163802,0.9133966,0.000034299337,0.00008086072,0.00019492536,0.00015657407,0.07589774,0.002898125,0.0054587657,0.0017384612,0.000040160496],"about_ca_topic_score_codex":0.0107294675,"about_ca_topic_score_gemma":0.025452992,"teacher_disagreement_score":0.0107294675,"about_ca_system_score_codex":0.00053476216,"about_ca_system_score_gemma":0.00047106462,"threshold_uncertainty_score":0.021333992},"labels":[],"label_agreement":null},{"id":"W1905277138","doi":"10.3847/0004-637x/817/2/86","title":"STAR-FORMING BRIGHTEST CLUSTER GALAXIES AT 0.25 &lt; z &lt; 1.25: A TRANSITIONING FUEL SUPPLY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Space Telescope Science Institute; University of Chicago; National Science Foundation","keywords":"Galaxy; Galaxy cluster; Cluster (spacecraft); Brightest cluster galaxy; Star formation; Luminosity; Spectroscopy","score_opus":0.006355785191123952,"score_gpt":0.19860945644174163,"score_spread":0.19225367125061768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1905277138","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996537,0.000026544396,0.00002096381,0.000016078831,6.4283796e-7,8.860865e-7,0.00009818968,0.000005039579,0.00017800146],"genre_scores_gemma":[0.9998184,0.000007816997,0.000010799663,0.000004018434,0.0000015903562,4.981228e-7,0.000094478964,7.440476e-7,0.000061763596],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986076,0.000010374377,0.0000059171257,0.00002953807,0.0000248005,0.000068497015],"domain_scores_gemma":[0.9992448,0.000053101783,0.000300676,0.000040178005,0.0000756652,0.00028566507],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001980399,0.0001676489,0.00031668015,0.0013365995,0.00040547983,0.00069253414,0.00035361102,0.00023434663,0.0016171733],"category_scores_gemma":[0.0005218484,0.00014672926,0.00020866354,0.00064632803,0.00055770646,0.00028894618,0.0005054994,0.0002428667,0.0003193832],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010307761,0.000014945738,0.9954572,0.00000388117,0.00001640512,0.000104381514,0.0001798971,0.00005837792,0.002661127,0.000060868824,0.00011045701,0.0012293889],"study_design_scores_gemma":[8.669282e-7,0.000009019257,0.999723,4.439159e-7,0.0000028266556,0.00002299097,0.000060385224,0.00002972785,0.000104358005,0.0000066498824,0.00003881901,7.723527e-7],"about_ca_topic_score_codex":0.01111492,"about_ca_topic_score_gemma":0.011552644,"teacher_disagreement_score":0.01111492,"about_ca_system_score_codex":0.0003747338,"about_ca_system_score_gemma":0.00014059094,"threshold_uncertainty_score":0.022100449},"labels":[],"label_agreement":null},{"id":"W1907854611","doi":"10.1088/0004-637x/813/2/104","title":"<i>KEPLER</i>MONITORING OF AN L DWARF. II. CLOUDS WITH MULTI-YEAR LIFETIMES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Light curve; Amplitude; Brown dwarf; Phase (matter); Spitzer Space Telescope; Kepler; Stars","score_opus":0.021636822064589053,"score_gpt":0.24978085516368576,"score_spread":0.2281440330990967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1907854611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941057,0.00047631294,0.00078138476,0.00008308827,0.000009259275,0.00000960525,0.0012983677,0.00011145798,0.0031247525],"genre_scores_gemma":[0.9958728,0.00013246725,0.0012726573,0.000050741375,0.000019418916,0.0000075794114,0.0017259785,0.000015150028,0.0009030278],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999379,0.0000025643847,0.0000039082292,0.000020310703,0.000015638703,0.000019668769],"domain_scores_gemma":[0.9997986,0.000021605007,0.000079224636,0.00002147641,0.000025574793,0.000053446598],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001319706,0.00011064505,0.00013839944,0.0013281027,0.00042783958,0.00037391752,0.00026522778,0.0003319571,0.00081558706],"category_scores_gemma":[0.00026130662,0.00009354506,0.0001255551,0.0005407028,0.00014164684,0.00042201963,0.00045123146,0.00024501648,0.00034487867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079370325,0.00017074635,0.7847996,0.00015170369,0.00009922554,0.0015916737,0.00045586372,0.0026320051,0.15041925,0.0005382915,0.003571547,0.05477633],"study_design_scores_gemma":[0.000015131419,0.00016156088,0.97332054,0.000021513777,0.000030341222,0.0015836526,0.00018531988,0.0021834758,0.016796608,0.000252211,0.005429424,0.000020222602],"about_ca_topic_score_codex":0.0028929957,"about_ca_topic_score_gemma":0.00708544,"teacher_disagreement_score":0.0028929957,"about_ca_system_score_codex":0.00032826304,"about_ca_system_score_gemma":0.00010519879,"threshold_uncertainty_score":0.0057522655},"labels":[],"label_agreement":null},{"id":"W1912369853","doi":"10.3847/0004-637x/819/2/163","title":"COSMIC VARIANCE IN THE NANOHERTZ GRAVITATIONAL WAVE BACKGROUND","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Gravitational wave background; Amplitude; Gravitational wave; Cosmic variance; Scaling; Planck; COSMIC cancer database; Range (aeronautics); Poisson distribution","score_opus":0.013544794107562683,"score_gpt":0.22593826131853917,"score_spread":0.2123934672109765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1912369853","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898935,0.000034507186,0.00848774,0.00012928262,0.00000953026,0.000007726088,0.00025077414,0.000079795675,0.0011070902],"genre_scores_gemma":[0.998933,0.000012801248,0.0007101551,0.000018963403,0.0000050320427,0.000005624329,0.00020114209,0.000015332123,0.00009784119],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995436,0.0001561383,0.000019249355,0.00012565234,0.00009573386,0.000059621063],"domain_scores_gemma":[0.99614304,0.002190222,0.0005873984,0.00054455985,0.00033803075,0.00019670412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015469873,0.00022648986,0.0002797753,0.0006054117,0.0003554771,0.0009993517,0.0006814993,0.00046212738,0.0011670396],"category_scores_gemma":[0.009746909,0.00021603303,0.0003424258,0.0005220056,0.0006410845,0.00094261684,0.00046425572,0.00046454574,0.00015024816],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016792893,0.00012142773,0.14049645,0.000042217387,0.00018391902,0.00017755174,0.00011275452,0.81988984,0.0064516966,0.026262505,0.0009231574,0.0051705036],"study_design_scores_gemma":[0.000023398203,0.00003065706,0.034167893,0.000006220356,0.000014867584,0.00003746732,0.000024816023,0.95559824,0.0016847551,0.008086207,0.00030165343,0.000023818813],"about_ca_topic_score_codex":0.0044398014,"about_ca_topic_score_gemma":0.003622021,"teacher_disagreement_score":0.0044398014,"about_ca_system_score_codex":0.00078335404,"about_ca_system_score_gemma":0.00030401186,"threshold_uncertainty_score":0.008827925},"labels":[],"label_agreement":null},{"id":"W1912953289","doi":"10.1088/0004-637x/808/2/130","title":"HUNTING FOR ORPHANED CENTRAL COMPACT OBJECTS AMONG RADIO PULSARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Physics; Astrophysics; Neutron star; Supernova; Luminosity; Galactic plane; Astronomy; Dipole; Accretion (finance); Millisecond pulsar; Magnetic field; Stars; Galaxy","score_opus":0.02349779506648467,"score_gpt":0.3211803976912633,"score_spread":0.2976826026247786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1912953289","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994918,0.00009235371,0.00013872239,0.000005480281,0.000001596216,0.0000039560337,0.0000311875,0.0000029018217,0.0002319707],"genre_scores_gemma":[0.9990963,0.00010754892,0.00036746013,0.000010674336,0.000007672029,0.0000034293214,0.00016833517,0.0000018474502,0.00023682468],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987376,0.000015029711,0.000008259308,0.00003781003,0.000019893423,0.000045309167],"domain_scores_gemma":[0.99942327,0.00009178729,0.00023607696,0.00006931296,0.000037622896,0.00014198733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002232141,0.00019388233,0.00027084947,0.0009837385,0.00055553473,0.00055751513,0.00033261665,0.00019954049,0.001443323],"category_scores_gemma":[0.00062557677,0.000097735254,0.0001583533,0.0005915161,0.00041706883,0.0003524146,0.00059141574,0.00013155711,0.00025099813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000115205745,0.000029784496,0.9832397,0.000017505377,0.000022260567,0.00068889296,0.0004562385,0.000048427424,0.0060076034,0.00024448184,0.0001011845,0.0090287905],"study_design_scores_gemma":[0.000008298946,0.00019722538,0.9919974,0.000015352949,0.00005079408,0.002314725,0.0010929247,0.00036600314,0.001554341,0.0003938405,0.0020001426,0.000008850677],"about_ca_topic_score_codex":0.0007712429,"about_ca_topic_score_gemma":0.0015313653,"teacher_disagreement_score":0.001443323,"about_ca_system_score_codex":0.000091928116,"about_ca_system_score_gemma":0.000094473064,"threshold_uncertainty_score":0.0048283935},"labels":[],"label_agreement":null},{"id":"W1917734344","doi":"10.1088/0004-637x/813/1/44","title":"SAGITTARIUS II, DRACO II AND LAEVENS 3: THREE NEW MILKY WAY SATELLITES DISCOVERED IN THE PAN-STARRS 1 3<i>π</i>SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":239,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Centre National de la Recherche Scientifique; Queen's University; University of Edinburgh; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Université de Strasbourg; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Globular cluster; Milky Way; Sagittarius; Dwarf galaxy; Astronomy; Astrophysics; Dwarf spheroidal galaxy; Local Group; Galaxy; Star cluster; Interacting galaxy","score_opus":0.027969701022397327,"score_gpt":0.2405659122229727,"score_spread":0.21259621120057537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1917734344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980064,0.00020696847,0.00008292586,0.000043541033,0.0000048404763,0.0000056673,0.00023167455,0.000016271071,0.0014017615],"genre_scores_gemma":[0.9977424,0.00014050414,0.00045382616,0.000063573374,0.000012759436,0.0000059266426,0.0011223273,0.0000053017566,0.00045334166],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998797,0.00000777896,0.000008962242,0.00003117052,0.00003641007,0.00003598557],"domain_scores_gemma":[0.99944323,0.000032263997,0.0002472829,0.000043274827,0.000040890827,0.00019295953],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014433128,0.00018701797,0.0001700531,0.0010244015,0.0004124211,0.0007000497,0.00023332711,0.00023982745,0.0007452268],"category_scores_gemma":[0.00033157784,0.00011894552,0.00016393955,0.00070145144,0.00044998326,0.00032583508,0.0010346003,0.0002276477,0.00017456447],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001750583,0.00002571207,0.97374356,0.000029103048,0.000041710697,0.0009770917,0.00053182384,0.000080411286,0.013245651,0.00052083086,0.000592355,0.010036617],"study_design_scores_gemma":[0.000015087692,0.000062563886,0.9901148,0.000012211757,0.000029057755,0.0017874601,0.0004435042,0.00017754342,0.0012986877,0.00017076626,0.005879181,0.000009005003],"about_ca_topic_score_codex":0.004948669,"about_ca_topic_score_gemma":0.0149048455,"teacher_disagreement_score":0.004948669,"about_ca_system_score_codex":0.00038023922,"about_ca_system_score_gemma":0.00024891124,"threshold_uncertainty_score":0.009839714},"labels":[],"label_agreement":null},{"id":"W1919816219","doi":"10.1088/0004-637x/811/2/89","title":"THE Q/U IMAGING EXPERIMENT: POLARIZATION MEASUREMENTS OF THE GALACTIC PLANE AT 43 AND 95 GHz","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"CMB cold spot; Physics; Galactic plane; Astrophysics; Planck; QUIET; Cosmic microwave background; Polarization (electrochemistry); Spectral index; Cosmic variance; Galactic Center; Astronomy; Spectral line; Galaxy; Redshift; Optics; Anisotropy","score_opus":0.017947235399736864,"score_gpt":0.23193274166148292,"score_spread":0.21398550626174606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1919816219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98836553,0.00015953925,0.0032118678,0.000080098835,0.000019576548,0.000021814927,0.0041570365,0.00018871641,0.0037959293],"genre_scores_gemma":[0.9869421,0.0001519807,0.006453841,0.00009312792,0.00005022567,0.00003947212,0.005552356,0.00004593831,0.00067091634],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971503,0.000047136076,0.000011695716,0.00009879274,0.0000667155,0.0000606478],"domain_scores_gemma":[0.9996251,0.000045940644,0.00012903442,0.00008484208,0.000034141223,0.00008083289],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005371297,0.00025590003,0.00021862735,0.0009521596,0.00029087684,0.00054789404,0.00040841298,0.0003160034,0.0010830836],"category_scores_gemma":[0.0004579452,0.0002723506,0.0002599903,0.00095516205,0.0003343452,0.0003507125,0.0005044439,0.00034327366,0.00031719657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024955394,0.00066674,0.6884248,0.00016846898,0.00063616043,0.00075448863,0.00088056864,0.006783738,0.21064535,0.00293806,0.013965012,0.07164095],"study_design_scores_gemma":[0.00012828122,0.00018999059,0.97496706,0.000012292567,0.000106353524,0.00030496248,0.00010967075,0.003269959,0.013449815,0.00043563024,0.006988511,0.00003745349],"about_ca_topic_score_codex":0.0025348363,"about_ca_topic_score_gemma":0.005615327,"teacher_disagreement_score":0.0025348363,"about_ca_system_score_codex":0.00019071004,"about_ca_system_score_gemma":0.00017767685,"threshold_uncertainty_score":0.005040109},"labels":[],"label_agreement":null},{"id":"W1921283484","doi":"10.1088/0004-637x/812/1/34","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. X. PROPERTIES OF ULTRA-COMPACT DWARFS IN THE M87, M49, AND M60 REGIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Canadian Space Agency; Centro de Astrofísica y Tecnologías Afines; Institut Universitaire de France; Max-Planck-Gesellschaft; China Postdoctoral Science Foundation; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; National Natural Science Foundation of China; Canarie; Jet Propulsion Laboratory; Chinese Academy of Sciences South America Center for Astronomy; Canadian Foundation for AIDS Research; Smithsonian Institution; Alfred P. Sloan Foundation; Agence Nationale de la Recherche; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Virgo Cluster; Astronomy; Globular cluster; Elliptical galaxy; Dwarf galaxy; Star cluster; Galaxy; Galaxy cluster; Effective radius; Surface brightness","score_opus":0.05592641596053525,"score_gpt":0.24036892618944386,"score_spread":0.18444251022890862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1921283484","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5819017,0.0026217357,0.00049371104,0.0014629528,0.00009104465,0.00013674957,0.39552954,0.0004002337,0.01736235],"genre_scores_gemma":[0.66630137,0.0009560326,0.0011529739,0.00047937557,0.00004839306,0.0001939403,0.3158185,0.00007576068,0.014973753],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999874,0.000019142968,0.000009088786,0.000028371256,0.000033729673,0.00003564235],"domain_scores_gemma":[0.9994825,0.000030138333,0.0001173363,0.000052499414,0.00010966974,0.00020785833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035883856,0.00015272536,0.00016713385,0.0023409063,0.00037999154,0.00046292384,0.00043412534,0.00026121747,0.0046401587],"category_scores_gemma":[0.0008935308,0.00011278974,0.00020638685,0.0019668767,0.00011498698,0.00027479164,0.0009753652,0.00023239637,0.0014924429],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016205854,0.00004067204,0.8925151,0.000099407174,0.00012878435,0.000074041774,0.00039886,0.0002006074,0.00096132915,0.00074078864,0.083684534,0.020993724],"study_design_scores_gemma":[0.0000071322697,0.000005162952,0.98897165,0.000014394424,0.0000111175605,0.000034289136,0.00016769662,0.000046082107,0.000050403014,0.000059129245,0.0106306765,0.0000023157477],"about_ca_topic_score_codex":0.13386934,"about_ca_topic_score_gemma":0.20085426,"teacher_disagreement_score":0.13386934,"about_ca_system_score_codex":0.00056550663,"about_ca_system_score_gemma":0.00054682087,"threshold_uncertainty_score":0.26618028},"labels":[],"label_agreement":null},{"id":"W1922377317","doi":"10.1088/0004-637x/792/1/57","title":"RADIO FREQUENCY MODELS OF NOVAE IN ERUPTION. I. THE FREE-FREE PROCESS IN BIPOLAR MORPHOLOGIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geophysics and Sensor Technology","field":"Engineering","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Science and Technology Facilities Council","keywords":"Circular symmetry; Spherical model; Spherical shell; Nova (rocket); Light curve; Shell (structure); Phase (matter); Spherical geometry","score_opus":0.009307271111965491,"score_gpt":0.19943410502486003,"score_spread":0.19012683391289453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1922377317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7977312,0.0012321142,0.12715186,0.0022233848,0.00028884647,0.00008958566,0.0013455038,0.0006890411,0.06924844],"genre_scores_gemma":[0.98585504,0.00022860794,0.0018390164,0.000093907256,0.000067805806,0.000027301372,0.0003160463,0.00017867178,0.011393574],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988675,0.000026264921,0.0000061952915,0.00002599564,0.00002222291,0.00003262711],"domain_scores_gemma":[0.9990182,0.000408604,0.00016755855,0.00009500948,0.00011148678,0.0001991922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005636573,0.0005056922,0.00047295316,0.0007282874,0.0005719548,0.0012469563,0.0016250963,0.001821515,0.0050579123],"category_scores_gemma":[0.004112848,0.000589688,0.0008204534,0.0003848416,0.00082993595,0.0019411377,0.0006900418,0.0010211363,0.0011270022],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013776668,0.000060367394,0.009439138,0.00006224951,0.00005507648,0.00045112282,0.00048781824,0.7336123,0.0021254786,0.23394491,0.0072595025,0.012364139],"study_design_scores_gemma":[0.000044477805,0.00001926535,0.0048796334,0.00001372311,0.000016169053,0.0001562771,0.000048205944,0.94015795,0.000113831156,0.053256597,0.0012728786,0.000021008667],"about_ca_topic_score_codex":0.005378733,"about_ca_topic_score_gemma":0.004571941,"teacher_disagreement_score":0.005378733,"about_ca_system_score_codex":0.00090915046,"about_ca_system_score_gemma":0.00022063561,"threshold_uncertainty_score":0.016920388},"labels":[],"label_agreement":null},{"id":"W1924595303","doi":"10.1088/0004-637x/810/2/118","title":"<i>SPITZER</i>SECONDARY ECLIPSE OBSERVATIONS OF FIVE COOL GAS GIANT PLANETS AND EMPIRICAL TRENDS IN COOL PLANET EMISSION SPECTRA","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"","keywords":"Planet; Hot Jupiter; Gas giant; Giant planet; Eclipse; Atmosphere (unit); Exoplanet; Jupiter (rocket family)","score_opus":0.031396581150970625,"score_gpt":0.26252958849773206,"score_spread":0.23113300734676143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1924595303","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992884,0.000029407385,0.00013036966,0.0000060273924,0.0000010198072,0.0000015771856,0.00015002809,0.000015897169,0.00037727904],"genre_scores_gemma":[0.99912363,0.00002234778,0.00021982571,0.00000537829,0.0000038326657,0.0000022409724,0.0005176276,0.0000056968393,0.000099431934],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994075,0.000004916034,0.000004067226,0.000018028606,0.000014403587,0.000017781951],"domain_scores_gemma":[0.99961346,0.00006516716,0.00016653335,0.000034899564,0.000050780403,0.000069193724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014229055,0.00018071267,0.00016352037,0.0008287466,0.00029821083,0.00029820655,0.00018164016,0.00023866045,0.00082244625],"category_scores_gemma":[0.000518555,0.00014295966,0.00017843116,0.00034319088,0.00018852275,0.00026417966,0.00033530057,0.00019659105,0.0001807885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001576889,0.000024789557,0.9707108,0.000021281507,0.00004907472,0.00012999309,0.00024115991,0.0004105983,0.024159737,0.00004278736,0.00017822476,0.0038739599],"study_design_scores_gemma":[0.000002347829,0.000033601653,0.99763155,0.0000013555652,0.00001096168,0.00011233509,0.00003481808,0.0003381306,0.0015591655,0.000013437181,0.00026044098,0.000001809075],"about_ca_topic_score_codex":0.0028106624,"about_ca_topic_score_gemma":0.0065565086,"teacher_disagreement_score":0.0028106624,"about_ca_system_score_codex":0.00023197665,"about_ca_system_score_gemma":0.000054944107,"threshold_uncertainty_score":0.005588591},"labels":[],"label_agreement":null},{"id":"W1927899762","doi":"10.1088/0004-637x/811/1/34","title":"EXPLORING THE ROLE OF GLOBULAR CLUSTER SPECIFIC FREQUENCY ON THE NOVA RATES IN THREE VIRGO ELLIPTICAL GALAXIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Nova (rocket); Globular cluster; Galaxy; Elliptical galaxy; Virgo Cluster; Dwarf nova","score_opus":0.07285185472062326,"score_gpt":0.24694059297490334,"score_spread":0.17408873825428006,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1927899762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99973494,0.000045537123,0.000052136027,0.0000041791654,3.7824216e-7,0.000001587546,0.000023529597,0.0000025899928,0.00013514908],"genre_scores_gemma":[0.99980277,0.00002017565,0.00006911436,0.0000026387374,0.0000012355689,0.0000016737266,0.000059356847,0.0000012237913,0.00004179332],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997627,0.000052624328,0.000018663644,0.00007047503,0.00004198347,0.000053481952],"domain_scores_gemma":[0.9979285,0.00074832345,0.00054511754,0.00019832021,0.00017835556,0.00040145544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00079315226,0.00023072374,0.00029404066,0.0019601255,0.000355148,0.00053714996,0.00037027785,0.0003909177,0.0003189897],"category_scores_gemma":[0.0024083538,0.00022404222,0.00034552568,0.0005562996,0.00046101242,0.00034876383,0.00070378394,0.000293372,0.00009208227],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017954879,0.000032154534,0.9838154,0.000009278451,0.00004840663,0.00011221611,0.00019277126,0.00044301333,0.012202256,0.00010626739,0.000016377071,0.0028421925],"study_design_scores_gemma":[0.0000012858666,0.000022344202,0.9989084,9.617635e-7,0.00000820978,0.00005807917,0.000046121764,0.00048228854,0.00041708056,0.000023986695,0.00002873546,0.0000026015875],"about_ca_topic_score_codex":0.0030842726,"about_ca_topic_score_gemma":0.0035730717,"teacher_disagreement_score":0.0030842726,"about_ca_system_score_codex":0.00053064886,"about_ca_system_score_gemma":0.000104770326,"threshold_uncertainty_score":0.0061326623},"labels":[],"label_agreement":null},{"id":"W1931408582","doi":"10.1086/339800","title":"Near-Infrared Adaptive Optics Spectroscopy of Binary Brown Dwarfs HD 130948B and HD 130948C","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Physics; Spectroscopy; Astrophysics; Adaptive optics; Subaru Telescope; Stellar classification; Infrared; Astronomy; Binary number; Laser guide star; Telescope; Circumbinary planet; Infrared spectroscopy; Spectral line; Stars; Spectrograph","score_opus":0.015459108912241547,"score_gpt":0.21895930527885166,"score_spread":0.2035001963666101,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1931408582","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917513,0.000040394232,0.00007979544,0.000009525674,0.000001168253,0.0000019654224,0.000062478844,0.000010256384,0.00061928993],"genre_scores_gemma":[0.9988524,0.000028642795,0.0005017288,0.000009681812,0.0000032629232,0.0000036598985,0.00027721346,0.0000027993285,0.00032062246],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992037,0.0000056255785,0.0000035436963,0.000027326756,0.000024009667,0.000019096444],"domain_scores_gemma":[0.9998493,0.000017340439,0.00004466496,0.000016166583,0.000025010582,0.000047413025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012051867,0.00014562646,0.00015510285,0.00084401923,0.00042752892,0.00019587667,0.00028919947,0.0002596249,0.0008135089],"category_scores_gemma":[0.00021028152,0.00010556357,0.00007946541,0.00036240433,0.00016110847,0.000143112,0.00034191983,0.00019217582,0.00016610182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005223463,0.0002902469,0.5154052,0.00005546469,0.0000699852,0.0007078759,0.0005700079,0.0005179839,0.45396015,0.00068604184,0.00081147376,0.026403347],"study_design_scores_gemma":[0.00002315418,0.00012613976,0.9857976,0.000003862237,0.000026718142,0.00068613776,0.0001250615,0.0009244954,0.011299636,0.00017788049,0.00080135703,0.000008027429],"about_ca_topic_score_codex":0.0019535366,"about_ca_topic_score_gemma":0.0028826634,"teacher_disagreement_score":0.0019535366,"about_ca_system_score_codex":0.00020337537,"about_ca_system_score_gemma":0.00006275506,"threshold_uncertainty_score":0.0038843155},"labels":[],"label_agreement":null},{"id":"W1931542633","doi":"10.3847/0004-637x/818/1/30","title":"THE SLOAN DIGITAL SKY SURVEY REVERBERATION MAPPING PROJECT: FIRST BROAD-LINE Hβ AND Mg ii LAGS AT z ≳ 0.3 FROM SIX-MONTH SPECTROSCOPY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Peking University; U.S. Department of Energy; National Natural Science Foundation of China; York University; Space Telescope Science Institute; Science and Technology Facilities Council; Carnegie Mellon University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; American Academy of Periodontology Foundation; China Scholarship Council; National Aeronautics and Space Administration","keywords":"Quasar; Reverberation mapping; Sky; Redshift; Spectroscopy; Black hole (networking); Spectral line; Lag","score_opus":0.017118365762298502,"score_gpt":0.23209655549151562,"score_spread":0.21497818972921712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1931542633","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9837482,0.00016603971,0.0017697494,0.00011907984,0.000018131852,0.00003622066,0.01182086,0.0001988105,0.0021227985],"genre_scores_gemma":[0.94885564,0.0001609655,0.0081789,0.0000890104,0.00004596783,0.000051880354,0.04099011,0.00011458225,0.0015128558],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959713,0.000058984937,0.000025760059,0.00006732322,0.0001550409,0.00009577543],"domain_scores_gemma":[0.9982242,0.00009893323,0.00052092574,0.0002734157,0.0004060872,0.0004763239],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014199439,0.00047371676,0.00022297882,0.0014510521,0.00034243314,0.0007649252,0.00030077633,0.00026212557,0.0008791307],"category_scores_gemma":[0.0009169766,0.00024565903,0.00029926377,0.0009962351,0.0002004543,0.0004261741,0.0010608439,0.00042981262,0.00063594355],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041898864,0.00021400314,0.94916075,0.00006140596,0.00015387131,0.00030635128,0.0004916778,0.0009239268,0.016835067,0.00021188465,0.0056350445,0.025587091],"study_design_scores_gemma":[0.000008321026,0.000037985737,0.9950865,0.000005152295,0.000011945449,0.000047706893,0.00005975288,0.00038234532,0.0013029913,0.000029758927,0.0030223124,0.0000051886755],"about_ca_topic_score_codex":0.010961273,"about_ca_topic_score_gemma":0.025796121,"teacher_disagreement_score":0.010961273,"about_ca_system_score_codex":0.00029632924,"about_ca_system_score_gemma":0.00042253063,"threshold_uncertainty_score":0.021794915},"labels":[],"label_agreement":null},{"id":"W1932008066","doi":"10.1088/0004-637x/776/1/15","title":"A COMBINED VERY LARGE TELESCOPE AND GEMINI STUDY OF THE ATMOSPHERE OF THE DIRECTLY IMAGED PLANET, β PICTORIS b","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Planet; Brown dwarf; Exoplanet; Effective temperature; Planetary mass; Planetary system; Astronomy; Stars","score_opus":0.005595558479575287,"score_gpt":0.19723193780379558,"score_spread":0.19163637932422029,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1932008066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99438196,0.00019633016,0.0015381478,0.000044990353,0.000006524621,0.000012665653,0.000528325,0.0000961522,0.0031948776],"genre_scores_gemma":[0.9945422,0.00015555628,0.0032996782,0.00003060355,0.000026275848,0.000010711357,0.001265007,0.000043615833,0.00062641164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999348,0.000009103895,0.0000021874118,0.000025476758,0.000013805078,0.00001464033],"domain_scores_gemma":[0.999859,0.000021999074,0.00003450131,0.00002801969,0.00001821024,0.00003830985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000179935,0.00025560646,0.00016340174,0.0006633274,0.00040755235,0.00044678317,0.00024490413,0.00019747365,0.0006079288],"category_scores_gemma":[0.0002494491,0.00024610633,0.00029597207,0.0005550708,0.00018398481,0.00038375668,0.00039092815,0.00029858292,0.00027510253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037038873,0.00025534423,0.7702369,0.00012983281,0.0002533605,0.0009608701,0.0011014928,0.010425493,0.17115885,0.0016321306,0.0019606238,0.0415147],"study_design_scores_gemma":[0.000011110868,0.000046891953,0.98586005,0.000005767173,0.00003483189,0.0002033976,0.00011741859,0.0094170505,0.0022161729,0.00019301241,0.0018867376,0.000007664675],"about_ca_topic_score_codex":0.0057357997,"about_ca_topic_score_gemma":0.006048044,"teacher_disagreement_score":0.0057357997,"about_ca_system_score_codex":0.00029998107,"about_ca_system_score_gemma":0.00016766984,"threshold_uncertainty_score":0.011404872},"labels":[],"label_agreement":null},{"id":"W1935338788","doi":"10.3847/0004-637x/818/2/132","title":"QUANTIFYING DISCORDANCE IN THE 2015 PLANCK CMB SPECTRUM","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":213,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Cosmic microwave background; Planck; Hubble's law; Spectral density; Matter power spectrum; Cosmic background radiation; Anisotropy; Baryon acoustic oscillations; Cold dark matter; Weak gravitational lensing","score_opus":0.016297194504215722,"score_gpt":0.2811750272503131,"score_spread":0.2648778327460974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1935338788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9881484,0.00030796858,0.0021651236,0.00034977644,0.00003349913,0.0000061920264,0.0019798677,0.00006542538,0.0069437614],"genre_scores_gemma":[0.99878365,0.00003807843,0.00030483448,0.00002685724,0.000011695544,0.0000028295312,0.0007396061,0.000013495527,0.0000790157],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99792165,0.0005697946,0.00017173644,0.0006620051,0.00054594385,0.00012890351],"domain_scores_gemma":[0.9868274,0.0046417103,0.003240459,0.0033032813,0.001566767,0.00042048865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0042614024,0.0001622652,0.00022128026,0.002065646,0.00046348525,0.0014915705,0.00054105284,0.00043071678,0.0022959197],"category_scores_gemma":[0.023856372,0.00016324522,0.00017797238,0.0020765471,0.0010129755,0.0012088548,0.0018157259,0.00037462683,0.00040582055],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027275653,0.000024440447,0.9426189,0.000113269794,0.00031942665,0.00013482073,0.004408626,0.004198744,0.003775887,0.011377012,0.0036852576,0.029070882],"study_design_scores_gemma":[0.0000029525797,0.00001406884,0.98982096,0.000037351154,0.000022467131,0.00006259998,0.0006587381,0.0016002702,0.0015652713,0.0024307792,0.0037562642,0.000028214465],"about_ca_topic_score_codex":0.003953302,"about_ca_topic_score_gemma":0.0025952058,"teacher_disagreement_score":0.0042614024,"about_ca_system_score_codex":0.0006700069,"about_ca_system_score_gemma":0.00020059063,"threshold_uncertainty_score":0.022536755},"labels":[],"label_agreement":null},{"id":"W1936097296","doi":"10.1088/0004-637x/814/1/32","title":"DIRECT IMAGING OF AN ASYMMETRIC DEBRIS DISK IN THE HD 106906 PLANETARY SYSTEM","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Université de Montréal; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Science Mission Directorate; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Physics; Debris disk; Planet; Astrophysics; Astronomy; Debris; Planetary system; Primary (astronomy)","score_opus":0.013213163237684724,"score_gpt":0.22479320596635463,"score_spread":0.2115800427286699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1936097296","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99474746,0.00024430198,0.00044404835,0.00005530586,0.000008639015,0.000006229206,0.00038966676,0.000045761706,0.0040584914],"genre_scores_gemma":[0.9982241,0.000063258594,0.0009619923,0.000033978085,0.000008052051,0.0000019828096,0.0003079318,0.000006023213,0.00039266242],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999553,0.0000026226905,0.000002243728,0.000013655993,0.000015384596,0.000010744011],"domain_scores_gemma":[0.9999083,0.000006882529,0.00002393033,0.0000136132885,0.000012880275,0.00003433207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006393569,0.00012051948,0.000097078184,0.00043577424,0.00026830626,0.00028311033,0.0001721945,0.00021716185,0.0012890041],"category_scores_gemma":[0.000110428125,0.00013749315,0.0000848489,0.00023396735,0.00014111219,0.00014525506,0.00037814118,0.00016756084,0.0004784806],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028196775,0.00008980457,0.20498994,0.00014226726,0.00004955035,0.0021865778,0.0004623781,0.00032536895,0.7743249,0.0004782354,0.0013885665,0.015280347],"study_design_scores_gemma":[0.000018505854,0.00015199254,0.96610147,0.000020543861,0.000025583126,0.0057374653,0.00031909128,0.001009817,0.021901324,0.00022816347,0.0044778576,0.000008127133],"about_ca_topic_score_codex":0.00072142977,"about_ca_topic_score_gemma":0.001653229,"teacher_disagreement_score":0.0012890041,"about_ca_system_score_codex":0.00012416556,"about_ca_system_score_gemma":0.00006340376,"threshold_uncertainty_score":0.0043121576},"labels":[],"label_agreement":null},{"id":"W1939777949","doi":"10.1088/0004-637x/765/2/87","title":"CONCURRENT SUPERMASSIVE BLACK HOLE AND GALAXY GROWTH: LINKING ENVIRONMENT AND NUCLEAR ACTIVITY IN<i>z</i>= 2.23 Hα EMITTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Leverhulme Trust","keywords":"Physics; Astrophysics; Supermassive black hole; Active galactic nucleus; QSOS; Galaxy; Star formation; Accretion (finance); Astronomy; Quasar","score_opus":0.006209695872673486,"score_gpt":0.18673766521836463,"score_spread":0.18052796934569115,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1939777949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996661,0.00002621946,0.000024014114,0.000014635154,4.9696894e-7,0.0000018119899,0.000090409405,0.0000024693313,0.00017382269],"genre_scores_gemma":[0.99969316,0.00002838504,0.000052446318,0.000013034593,0.0000037094248,0.0000026845355,0.00011281604,0.0000018725464,0.00009182652],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999248,0.000007635264,0.000004425924,0.000020523627,0.000013507687,0.000029124976],"domain_scores_gemma":[0.99931264,0.000058883747,0.00030088917,0.000038454647,0.000037976533,0.00025112508],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012827749,0.00016508748,0.00015608234,0.00062592805,0.00024107323,0.0006024385,0.0002523705,0.00030664567,0.0010764992],"category_scores_gemma":[0.00047359915,0.00014168548,0.0001392287,0.00043899365,0.00038749253,0.0002821734,0.00045880768,0.00036443665,0.00022597003],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017395812,0.000061086714,0.98718387,0.000003994222,0.000015058202,0.00018480045,0.00013447879,0.000051787087,0.01088104,0.000048308542,0.00005217674,0.0012094466],"study_design_scores_gemma":[0.0000017395721,0.000019058867,0.9994337,4.1633152e-7,0.0000034121654,0.00012701494,0.00006126446,0.000049971746,0.00023910568,0.000015375765,0.000047784615,0.0000011710463],"about_ca_topic_score_codex":0.006559022,"about_ca_topic_score_gemma":0.011218544,"teacher_disagreement_score":0.006559022,"about_ca_system_score_codex":0.00024340359,"about_ca_system_score_gemma":0.00017690701,"threshold_uncertainty_score":0.013041675},"labels":[],"label_agreement":null},{"id":"W1940085570","doi":"10.3847/0004-637x/816/2/48","title":"THE PHASE SPACE OF SpARCS CLUSTERS: USING HERSCHEL TO PROBE DUST TEMPERATURE AS A FUNCTION OF ENVIRONMENT AND ACCRETION HISTORY*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Waterloo; University of Toronto","funders":"","keywords":"Accretion (finance); Galaxy; Galaxy cluster; Star formation; Cluster (spacecraft); Brightest cluster galaxy; Galaxy formation and evolution; Galaxy merger","score_opus":0.009621539194571791,"score_gpt":0.21225005647965078,"score_spread":0.202628517285079,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1940085570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991504,0.000017413337,0.00012005271,0.000005546085,4.685603e-7,0.0000027062758,0.00040868888,0.000011248064,0.00028347064],"genre_scores_gemma":[0.99821365,0.000014070535,0.00040341337,0.000007480934,0.0000026121372,0.0000038575154,0.0011454521,0.000005683503,0.00020383409],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998965,0.000017838163,0.0000034764312,0.000036352878,0.000021114909,0.0000246827],"domain_scores_gemma":[0.9995449,0.00007709988,0.0001405498,0.00007889303,0.00007486772,0.00008364971],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027890975,0.00013540531,0.00016630656,0.0006832985,0.00030703825,0.00038677477,0.00019714705,0.00012023675,0.00076566875],"category_scores_gemma":[0.0005141356,0.00010014496,0.00014767151,0.0005216375,0.00021042954,0.0002934036,0.00031392724,0.00013297421,0.00020623479],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034989812,0.00010779959,0.96764207,0.00001681402,0.00007904082,0.00008193479,0.00040911627,0.004617687,0.018833442,0.00038804798,0.00042920202,0.0070448387],"study_design_scores_gemma":[0.000008513213,0.00004723372,0.994263,0.0000013096062,0.000005657264,0.000036240705,0.00010418622,0.0035240566,0.001454688,0.00007092243,0.0004779774,0.0000061042565],"about_ca_topic_score_codex":0.014238311,"about_ca_topic_score_gemma":0.024026502,"teacher_disagreement_score":0.014238311,"about_ca_system_score_codex":0.0004401747,"about_ca_system_score_gemma":0.00020488653,"threshold_uncertainty_score":0.028310835},"labels":[],"label_agreement":null},{"id":"W1941341701","doi":"10.1088/0004-637x/814/1/17","title":"<i>SPITZER</i>IMAGING OF STRONGLY LENSED<i>HERSCHEL</i>-SELECTED DUSTY STAR-FORMING GALAXIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"Key Programme; Jet Propulsion Laboratory; National Research Foundation; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; National Science Foundation","keywords":"Galaxy; Flux (metallurgy); Star formation; Spectral energy distribution; Galaxy formation and evolution; Luminous infrared galaxy; Adaptive optics; Stellar mass","score_opus":0.011288594183912167,"score_gpt":0.2162175702250648,"score_spread":0.20492897604115262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1941341701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99656004,0.00008461606,0.00034181835,0.000026747455,0.0000015454093,0.000002732547,0.0009165837,0.000107161686,0.001958724],"genre_scores_gemma":[0.99607605,0.00008375314,0.0012112454,0.000035720936,0.000008849609,0.0000032891403,0.0020094793,0.000022238199,0.00054925896],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999325,0.000004069657,0.0000029244816,0.00001839542,0.000017784347,0.00002424255],"domain_scores_gemma":[0.99986255,0.000010369787,0.000058223923,0.000013644808,0.000020564334,0.00003464258],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008949396,0.0001461923,0.00009727436,0.0012307668,0.00015603607,0.00027889566,0.0001656501,0.00015153977,0.0015184068],"category_scores_gemma":[0.000118975586,0.00007711565,0.00017382368,0.00044452105,0.00014192834,0.00015455426,0.00021972386,0.0001231603,0.0002581324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026272968,0.000075808,0.5837628,0.00007553391,0.00014956301,0.00047418903,0.00044616105,0.003614718,0.3820848,0.0005225053,0.0036394035,0.02489177],"study_design_scores_gemma":[0.0000056856697,0.000015470987,0.9903441,0.0000037873174,0.000012369698,0.00014696072,0.00004924366,0.0013631249,0.0069172103,0.000052441705,0.0010838091,0.0000058390883],"about_ca_topic_score_codex":0.008832561,"about_ca_topic_score_gemma":0.020308798,"teacher_disagreement_score":0.008832561,"about_ca_system_score_codex":0.0003772004,"about_ca_system_score_gemma":0.00008888441,"threshold_uncertainty_score":0.01756233},"labels":[],"label_agreement":null},{"id":"W1941419763","doi":"10.1088/0004-637x/810/2/153","title":"AN EXTENDED VIEW OF THE PISCES OVERDENSITY FROM THE SCUSS SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Chinese Academy of Sciences; U.S. Department of Energy; National Natural Science Foundation of China; York University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; College of Engineering, Michigan State University; Johns Hopkins University; National Key Research and Development Program of China; Science and Technology Facilities Council; Carnegie Mellon University; Harvard University; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Brookhaven National Laboratory; European Commission","keywords":"Milky Way; Halo; RR Lyrae variable; Stars; Galactic halo; Globular cluster; Local Group; Galaxy","score_opus":0.03645903036041086,"score_gpt":0.302779359804458,"score_spread":0.26632032944404715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1941419763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5947321,0.0046673175,0.004387257,0.0039925864,0.00022273479,0.00017134921,0.14189136,0.0021102491,0.24782509],"genre_scores_gemma":[0.90177774,0.0025118045,0.005473596,0.0005516071,0.00037077427,0.00009882644,0.063846506,0.00024974075,0.025119513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988246,0.000010027542,0.0000044527933,0.000022004879,0.000053983345,0.000027043447],"domain_scores_gemma":[0.9995363,0.000045569603,0.000079072524,0.000046483627,0.00018571052,0.000106829946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000096712654,0.0002211381,0.00011263626,0.003524018,0.00033856314,0.00059447624,0.0002720524,0.00018994439,0.015623923],"category_scores_gemma":[0.00041171172,0.000117637195,0.00019158963,0.0030896491,0.00019925131,0.00033100112,0.00084405474,0.00036984094,0.0019513996],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017999561,0.000049036837,0.5966973,0.00038337952,0.00009651759,0.0012714907,0.0023383873,0.0019045259,0.0062463926,0.0057052746,0.26581717,0.119310506],"study_design_scores_gemma":[0.000006825877,0.000012937375,0.88377297,0.00009516147,0.000009263975,0.00039676568,0.0005177944,0.00082594034,0.0003206063,0.00042116147,0.11361035,0.000010131552],"about_ca_topic_score_codex":0.10242536,"about_ca_topic_score_gemma":0.14450817,"teacher_disagreement_score":0.10242536,"about_ca_system_score_codex":0.00047965805,"about_ca_system_score_gemma":0.00050184206,"threshold_uncertainty_score":0.20365834},"labels":[],"label_agreement":null},{"id":"W1942076644","doi":"10.3847/0004-637x/820/2/108","title":"THE MIRA–TITAN UNIVERSE: PRECISION PREDICTIONS FOR DARK ENERGY SURVEYS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"","keywords":"Dark energy; Physics; Weak gravitational lensing; Cosmology; Matter power spectrum; Galaxy; Redshift; COSMIC cancer database; Astrophysics","score_opus":0.008145317984341937,"score_gpt":0.211674350008023,"score_spread":0.20352903202368108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1942076644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9069806,0.00023616882,0.086185165,0.00061634823,0.000021603199,0.00002938357,0.00037520798,0.0004195497,0.005135937],"genre_scores_gemma":[0.98605716,0.00003910051,0.013439143,0.00002473106,0.000008870028,0.000014607866,0.00015576674,0.000029763976,0.00023091039],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993291,0.00037287123,0.00001927612,0.00008769581,0.00013221671,0.00005887393],"domain_scores_gemma":[0.9880967,0.0076858094,0.00079171907,0.0024507958,0.00069860264,0.00027639375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00626714,0.00032343587,0.0003649453,0.0005070205,0.00041492342,0.0008314466,0.000731111,0.00044319584,0.00075755245],"category_scores_gemma":[0.031792473,0.0002902328,0.0003150549,0.00041802166,0.00084999454,0.0012093731,0.0008654774,0.00068413286,0.00011828927],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003325809,0.0000706154,0.057133734,0.000040731473,0.00008849253,0.00007150356,0.00024917285,0.8563196,0.0019937146,0.0684128,0.00086294726,0.014424039],"study_design_scores_gemma":[0.000023589237,0.000035742003,0.008855483,0.000016250184,0.000011443294,0.000018678535,0.000027374123,0.9655894,0.0015047744,0.023447372,0.0004561795,0.000013808394],"about_ca_topic_score_codex":0.0057261186,"about_ca_topic_score_gemma":0.0038159671,"teacher_disagreement_score":0.00626714,"about_ca_system_score_codex":0.00088287005,"about_ca_system_score_gemma":0.000505658,"threshold_uncertainty_score":0.033144236},"labels":[],"label_agreement":null},{"id":"W1943471801","doi":"10.1088/0004-637x/807/2/141","title":"GOODS-<i>HERSCHEL</i>: STAR FORMATION, DUST ATTENUATION, AND THE FIR–RADIO CORRELATION ON THE MAIN SEQUENCE OF STAR-FORMING GALAXIES UP TO<i>z</i>≃ 4","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":205,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"FP7 Space; Institut national des sciences de l'Univers; Science and Technology Facilities Council; Jet Propulsion Laboratory; Max-Planck-Institut für Astronomie; Centre National de la Recherche Scientifique; National Radio Astronomy Observatory; KU Leuven; National Astronomical Observatory of Japan; California Institute of Technology; European Commission; Agence Nationale de la Recherche; National Science Foundation; European Space Agency; National Aeronautics and Space Administration","keywords":"Galaxy; Redshift; Attenuation; Stellar mass; Star formation; COSMIC cancer database; Cosmic dust; Galaxy formation and evolution","score_opus":0.020022989207589832,"score_gpt":0.22717066519625614,"score_spread":0.20714767598866632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1943471801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959559,0.00008707566,0.00022140413,0.000033104763,0.0000017188281,0.0000024239314,0.00267781,0.00004342191,0.0009772532],"genre_scores_gemma":[0.99141204,0.000047417678,0.00066577544,0.000024175013,0.000008499113,0.00000451363,0.0073152413,0.000013144918,0.0005091438],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998536,0.000015749076,0.0000062763247,0.00005381268,0.000023652065,0.000046919562],"domain_scores_gemma":[0.9984378,0.0002597351,0.0007363776,0.00022190444,0.00011233093,0.00023178046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044364054,0.00027613895,0.00024184931,0.0014544812,0.00017335016,0.00055591244,0.00030102016,0.00023487073,0.0016955377],"category_scores_gemma":[0.0009108203,0.00016384249,0.00029134896,0.00085877004,0.000343928,0.00036011942,0.00059985655,0.00023126931,0.00054106524],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010352694,0.000028249862,0.98627687,0.000022559836,0.000081522354,0.000086772154,0.000078909434,0.0015464037,0.0067884624,0.0002547264,0.0005773256,0.004154798],"study_design_scores_gemma":[0.0000028135266,0.000008324692,0.99848384,0.0000022081645,0.000008081799,0.000029030247,0.0000117229165,0.00048720182,0.00052165694,0.00004903395,0.00039386272,0.0000022670342],"about_ca_topic_score_codex":0.008060398,"about_ca_topic_score_gemma":0.011868573,"teacher_disagreement_score":0.008060398,"about_ca_system_score_codex":0.00042329906,"about_ca_system_score_gemma":0.00017569716,"threshold_uncertainty_score":0.016026974},"labels":[],"label_agreement":null},{"id":"W1947631097","doi":"10.1088/0004-637x/807/2/117","title":"MOLECULAR AND IONIZED HYDROGEN IN 30 DORADUS. I. IMAGING OBSERVATIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Hydrogen molecule; Ionization; Hydrogen; Physics; Astrophysics; Astronomy; Ion; Quantum mechanics","score_opus":0.02008573906683345,"score_gpt":0.2454062366794904,"score_spread":0.22532049761265696,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1947631097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99566144,0.0003061111,0.00025256825,0.000038067392,0.000005426618,0.000013998176,0.00075637817,0.00004111974,0.0029248192],"genre_scores_gemma":[0.9950655,0.00018199692,0.0018271029,0.00006495243,0.000015800717,0.000015925827,0.0021438517,0.000016738742,0.0006681779],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991393,0.000005365007,0.0000034319678,0.000025466705,0.000027147507,0.000024600431],"domain_scores_gemma":[0.9999125,0.000004764872,0.000021601989,0.000009625544,0.000013277135,0.00003833975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099630124,0.00021421615,0.00025067982,0.0006303723,0.0003838847,0.0003231323,0.0003525742,0.00025654642,0.0007812399],"category_scores_gemma":[0.00010898573,0.00020843289,0.00017048138,0.0003656348,0.00017721088,0.00018394254,0.0005878104,0.00019057372,0.000251447],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058598915,0.00014617499,0.49167588,0.000194571,0.00012435441,0.0010589266,0.000981989,0.0014235029,0.46025681,0.00047802032,0.0019025735,0.041171223],"study_design_scores_gemma":[0.00001730469,0.00006406922,0.98868984,0.000010284583,0.000017161821,0.00049277506,0.00014268488,0.000674266,0.005271008,0.00005581325,0.004556479,0.0000082723645],"about_ca_topic_score_codex":0.0063264337,"about_ca_topic_score_gemma":0.013504989,"teacher_disagreement_score":0.0063264337,"about_ca_system_score_codex":0.00038055654,"about_ca_system_score_gemma":0.00019890623,"threshold_uncertainty_score":0.012579203},"labels":[],"label_agreement":null},{"id":"W1947931147","doi":"10.1088/0004-637x/808/1/69","title":"ALMA OBSERVATIONS OF THE LARGEST PROTO-PLANETARY DISK IN THE ORION NEBULA, 114–426: A CO SILHOUETTE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; National Research Council Canada","funders":"","keywords":"Astrophysics; Physics; Nebula; Protoplanetary disk; Orion Nebula; Formation and evolution of the Solar System; Molecular cloud; Absorption (acoustics); Mass ratio; Astronomy; Planet; Stars; Optics","score_opus":0.03181041989458088,"score_gpt":0.25706057647860275,"score_spread":0.22525015658402187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1947931147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973036,0.00014447092,0.00010230034,0.000028333132,0.0000055941377,0.0000068984896,0.0002886751,0.0000507368,0.0020693734],"genre_scores_gemma":[0.9982273,0.00006257645,0.00054103706,0.000012936209,0.000014167704,0.000005584334,0.0005287293,0.000007638837,0.0006000168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999244,0.000003757869,0.0000027311012,0.000027073253,0.000021893957,0.000020049374],"domain_scores_gemma":[0.9998735,0.000010722364,0.000025671476,0.000009274276,0.0000254717,0.000055356337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007198015,0.00021695449,0.00020027108,0.00080377335,0.0006600035,0.00049943436,0.0002876793,0.0003592474,0.0015536058],"category_scores_gemma":[0.00018786691,0.00014134731,0.00017912529,0.00036840275,0.00011686139,0.00022460517,0.00042111,0.00021744303,0.0002811374],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089128676,0.00029812302,0.69351494,0.00015874136,0.000119827586,0.0012369895,0.0010500588,0.0011796427,0.25293902,0.00030297143,0.0017418199,0.04656658],"study_design_scores_gemma":[0.000025577481,0.00015086922,0.9872729,0.00001502645,0.000053075415,0.00049256935,0.00017196697,0.0014065618,0.0054283123,0.000056487817,0.004915766,0.000010937887],"about_ca_topic_score_codex":0.0048227706,"about_ca_topic_score_gemma":0.010798045,"teacher_disagreement_score":0.0048227706,"about_ca_system_score_codex":0.00034265782,"about_ca_system_score_gemma":0.00011908091,"threshold_uncertainty_score":0.009589374},"labels":[],"label_agreement":null},{"id":"W1949047154","doi":"10.1088/0004-637x/810/2/150","title":"NANOGrav CONSTRAINTS ON GRAVITATIONAL WAVE BURSTS WITH MEMORY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Gravitational wave; Pulsar; Amplitude; Observatory; Neutron star; Gravitational-wave observatory; LIGO; Gravitation","score_opus":0.025747338694619298,"score_gpt":0.30839204107671664,"score_spread":0.2826447023820973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1949047154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9714957,0.0006999098,0.0031158244,0.0005475952,0.00003831634,0.000013735047,0.0010204666,0.000092725146,0.022975657],"genre_scores_gemma":[0.9962598,0.00020541724,0.0014119904,0.00018715637,0.000041381147,0.000013158674,0.00085856783,0.000018031993,0.001004591],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998062,0.000014257775,0.000012393018,0.000058156107,0.00006130681,0.000047712656],"domain_scores_gemma":[0.99738973,0.00093842286,0.00079349556,0.0004424566,0.00019894927,0.0002369158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005285207,0.00022804548,0.00018081816,0.0009859675,0.00044229522,0.0010621465,0.00045365965,0.00049933296,0.003232947],"category_scores_gemma":[0.0026771254,0.00027708174,0.00016392689,0.00082417345,0.00048507145,0.0011916516,0.0010451573,0.00042880134,0.0005260843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007689722,0.00024655735,0.73209566,0.00022908213,0.000114230555,0.0007400068,0.00074669824,0.0044983295,0.11309386,0.06373859,0.004343686,0.07938441],"study_design_scores_gemma":[0.00007059491,0.00023429707,0.8919075,0.000107276785,0.000078877594,0.0014603627,0.0004380428,0.02008413,0.02044125,0.036184553,0.028932584,0.000060489427],"about_ca_topic_score_codex":0.0011369284,"about_ca_topic_score_gemma":0.002912407,"teacher_disagreement_score":0.003232947,"about_ca_system_score_codex":0.0004183406,"about_ca_system_score_gemma":0.00019002573,"threshold_uncertainty_score":0.010815322},"labels":[],"label_agreement":null},{"id":"W1952407255","doi":"10.1088/0004-637x/806/2/166","title":"BROADBAND X-RAY PROPERTIES OF THE GAMMA-RAY BINARY 1FGL J1018.6–5856","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; X-ray; Astrophysics; Binary number; Gamma ray; Broadband; Astronomy; X-ray binary; Optics; Neutron star","score_opus":0.028296539429365646,"score_gpt":0.22503174556711383,"score_spread":0.1967352061377482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1952407255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982027,0.00027200565,0.00007753574,0.000028650793,0.0000073265383,0.000004116217,0.00025661683,0.000015734277,0.001135334],"genre_scores_gemma":[0.9982254,0.00009132116,0.0003002444,0.000037923564,0.000018744578,0.0000040860223,0.00089954893,0.000007788325,0.00041490942],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998361,0.000008341136,0.000012805468,0.000059521062,0.00004588299,0.00003734019],"domain_scores_gemma":[0.99952817,0.00004605348,0.0002143025,0.000035433146,0.000054509543,0.00012160907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027311116,0.0002822062,0.00055058405,0.001282918,0.0005447156,0.0007274346,0.00032468495,0.00045281023,0.0012304685],"category_scores_gemma":[0.0005891838,0.00028328854,0.00014581613,0.000716542,0.0002829363,0.00048976444,0.0006502421,0.00035401675,0.00067788933],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006520883,0.00033822283,0.83924997,0.00014139595,0.000098733064,0.001660715,0.0005164606,0.00104348,0.13167904,0.0003685471,0.0012259127,0.023025481],"study_design_scores_gemma":[0.000014065209,0.00013039174,0.9959686,0.000011375786,0.00001750604,0.00070729514,0.00008346751,0.00082425214,0.0012806959,0.000053540643,0.00089873746,0.00000998569],"about_ca_topic_score_codex":0.0022267958,"about_ca_topic_score_gemma":0.0046962146,"teacher_disagreement_score":0.0022267958,"about_ca_system_score_codex":0.00039969137,"about_ca_system_score_gemma":0.00011200851,"threshold_uncertainty_score":0.004427612},"labels":[],"label_agreement":null},{"id":"W1955284893","doi":"10.3847/0004-637x/816/1/44","title":"THE SENSITIVITY OF CORE-COLLAPSE SUPERNOVAE TO NUCLEAR ELECTRON CAPTURE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Supernova; Sensitivity (control systems); Electron capture; Luminosity; Range (aeronautics); Nuclear reaction; Neutron; Neutron capture","score_opus":0.014334857582282628,"score_gpt":0.23755402221580263,"score_spread":0.22321916463352,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1955284893","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98261124,0.00016237283,0.0142750675,0.000023285256,0.000006127021,0.00003734796,0.0007154056,0.00031957822,0.0018495935],"genre_scores_gemma":[0.9966859,0.00007964616,0.0016840242,0.000017373764,0.0000027900194,0.000024856645,0.0011887945,0.00004675392,0.00026996882],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99935335,0.00020365058,0.0000572077,0.0001299527,0.00019152761,0.00006425395],"domain_scores_gemma":[0.9957444,0.0024609242,0.0004942441,0.00073366804,0.00042184384,0.00014488488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026162523,0.00053757476,0.0004952578,0.001198863,0.00023720789,0.0006784064,0.0009247389,0.00031331193,0.0008157184],"category_scores_gemma":[0.0060534924,0.00035865762,0.00068933755,0.00052958674,0.00021854733,0.00044320954,0.00090985745,0.0003824423,0.0002066066],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012232641,0.0004291085,0.25667614,0.00022155164,0.0010553909,0.00019745034,0.000081931794,0.5097528,0.2021891,0.003195758,0.0005145098,0.024462951],"study_design_scores_gemma":[0.0000453044,0.00072929496,0.13708954,0.000022596825,0.00016823095,0.00025267634,0.00004562221,0.67363566,0.18544923,0.001425875,0.0010570597,0.00007888752],"about_ca_topic_score_codex":0.0032588465,"about_ca_topic_score_gemma":0.0017224787,"teacher_disagreement_score":0.0032588465,"about_ca_system_score_codex":0.00048535285,"about_ca_system_score_gemma":0.00022851846,"threshold_uncertainty_score":0.013836265},"labels":[],"label_agreement":null},{"id":"W1959851080","doi":"10.1088/0004-637x/727/1/54","title":"ANISOTROPIC ACTIVE GALACTIC NUCLEUS OUTFLOWS AND ENRICHMENT OF THE INTERGALACTIC MEDIUM. II. METALLICITY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Metallicity; Active galactic nucleus; Galaxy; Stars; Luminosity; Intergalactic travel; Anisotropy","score_opus":0.011321449914603541,"score_gpt":0.20911102520797453,"score_spread":0.197789575293371,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1959851080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977737,0.000045631106,0.0011508033,0.000037379985,0.000003715485,0.0000056857034,0.000076095486,0.000026051373,0.0008808655],"genre_scores_gemma":[0.9990018,0.00003336062,0.0006530114,0.000014013563,0.0000028417899,0.0000036918336,0.00007292859,0.00000894408,0.0002093549],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992347,0.000022845412,0.0000034525046,0.0000140647735,0.00001037193,0.00002581715],"domain_scores_gemma":[0.99968076,0.000095279356,0.00010812732,0.000036868198,0.000025182288,0.00005390707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002112616,0.00036991833,0.00021637524,0.00029136645,0.00023591775,0.00057077524,0.00051098457,0.00048011524,0.0009727839],"category_scores_gemma":[0.0011670231,0.00024823507,0.00045460594,0.00027945326,0.00037586782,0.00042498566,0.0004749077,0.00037057133,0.0000857949],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022392586,0.00012557293,0.11288747,0.000050221293,0.000115477196,0.00039385946,0.00010564694,0.8570039,0.022078559,0.004172079,0.0002177149,0.0026255331],"study_design_scores_gemma":[0.000094021634,0.00009754639,0.04071634,0.000009535741,0.000041565963,0.0000793829,0.000076606164,0.9518467,0.004731327,0.0018055347,0.0004858314,0.00001562519],"about_ca_topic_score_codex":0.007313107,"about_ca_topic_score_gemma":0.0058170715,"teacher_disagreement_score":0.007313107,"about_ca_system_score_codex":0.0007160747,"about_ca_system_score_gemma":0.00027451146,"threshold_uncertainty_score":0.01454109},"labels":[],"label_agreement":null},{"id":"W1960367046","doi":"10.1088/0004-637x/812/1/43","title":"HerMES: ALMA IMAGING OF<i>HERSCHEL</i>-SELECTED DUSTY STAR-FORMING GALAXIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Submillimeter Array; Astronomy; Redshift; Millimeter; Luminous infrared galaxy; Gravitational lens; Star formation; Point source; Flux (metallurgy)","score_opus":0.010425460737517158,"score_gpt":0.2194246902505677,"score_spread":0.20899922951305056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1960367046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75694877,0.0013421272,0.040757295,0.00094832736,0.0001916389,0.00036406095,0.10431082,0.019099813,0.07603716],"genre_scores_gemma":[0.799022,0.0006085874,0.10798465,0.00076287164,0.0004174308,0.00031113706,0.077215225,0.0013144962,0.012363627],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9996573,0.000032551503,0.000010648902,0.00011191688,0.00012794933,0.000059718328],"domain_scores_gemma":[0.99966145,0.000029087889,0.00006869588,0.00009747372,0.000064912,0.00007844621],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004974614,0.00033700696,0.00024777727,0.0017921986,0.00042213508,0.0008379978,0.0006095152,0.00035169718,0.0066816704],"category_scores_gemma":[0.00051287643,0.0002949245,0.00043994212,0.0008135143,0.00018689515,0.0006009383,0.0006782887,0.000412257,0.0022679241],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007546832,0.0004923697,0.23256433,0.00044135674,0.0006336256,0.00088006863,0.0012830477,0.011249089,0.33062026,0.010368442,0.2323543,0.17835842],"study_design_scores_gemma":[0.00019778893,0.00017726219,0.70776224,0.00008749169,0.00013896429,0.0010080758,0.00023340974,0.05253553,0.04034766,0.0031885554,0.19419926,0.00012385793],"about_ca_topic_score_codex":0.008004035,"about_ca_topic_score_gemma":0.018094134,"teacher_disagreement_score":0.008004035,"about_ca_system_score_codex":0.0004805271,"about_ca_system_score_gemma":0.00031468147,"threshold_uncertainty_score":0.022352457},"labels":[],"label_agreement":null},{"id":"W1963542719","doi":"10.1086/324536","title":"Eccentricity Evolution of Migrating Planets","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planetesimal; Planet; Physics; Planetary migration; Astrophysics; Angular momentum; Eccentricity (behavior); Protoplanetary disk; Debris disk; Planetary mass; Planetary system; Giant planet; Astronomy; Classical mechanics","score_opus":0.011799020799120454,"score_gpt":0.20427687905979885,"score_spread":0.1924778582606784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963542719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99863213,0.000028058934,0.0006387783,0.000010519472,9.3560465e-7,0.0000010966141,0.000015271375,0.000015094178,0.0006581314],"genre_scores_gemma":[0.9991091,0.000016745917,0.00060545845,0.0000016287706,5.725199e-7,0.0000011780983,0.00004654426,0.000008866098,0.0002099126],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999405,0.000007679874,0.000003264105,0.000019163675,0.0000134421425,0.00001600736],"domain_scores_gemma":[0.9995189,0.00015269135,0.00013170917,0.00004668202,0.00009179274,0.00005836015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018201221,0.00016437123,0.00019346057,0.0004405918,0.00027022863,0.00039061,0.00023957147,0.00026487347,0.0008091134],"category_scores_gemma":[0.00234913,0.00015809094,0.00016402164,0.000286522,0.0002744183,0.00030876225,0.0003535488,0.0002495426,0.00014734182],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065235957,0.00013241271,0.38569123,0.00009577417,0.00009980796,0.0012163238,0.0010203653,0.32509822,0.24705955,0.0071990606,0.0004896046,0.031245343],"study_design_scores_gemma":[0.000056610297,0.00036033176,0.2670003,0.000027424101,0.00007819585,0.001340888,0.0004474049,0.66526824,0.059706163,0.0032507756,0.0024081413,0.000055623514],"about_ca_topic_score_codex":0.001834328,"about_ca_topic_score_gemma":0.001288542,"teacher_disagreement_score":0.001834328,"about_ca_system_score_codex":0.00036251178,"about_ca_system_score_gemma":0.00011687721,"threshold_uncertainty_score":0.0036473274},"labels":[],"label_agreement":null},{"id":"W1963576527","doi":"10.1086/341335","title":"Molecular Gas in Candidate Double‐barred Galaxies. I. The Diverse Morphology and Dynamics of NGC 2273 and NGC 5728","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Bar (unit); Astronomy; Star formation; Stars; Dust lane; Hubble sequence; Luminous infrared galaxy","score_opus":0.006961701829114317,"score_gpt":0.19954157773967432,"score_spread":0.19257987591056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963576527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965715,0.000042567463,0.00005120772,0.0000057239577,7.940485e-7,0.0000014168411,0.000027418904,0.0000063335606,0.00020740059],"genre_scores_gemma":[0.99961805,0.000014991501,0.00013005112,0.000005120496,9.678718e-7,0.0000021087587,0.00010931848,0.000001502563,0.00011789367],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999176,0.0000048799493,0.0000038821545,0.000024422096,0.000019789124,0.000029306795],"domain_scores_gemma":[0.9997274,0.00002088368,0.00009711697,0.000020244903,0.000024932782,0.000109431836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011687954,0.00020740357,0.00019377441,0.00086656417,0.0002787282,0.00046814306,0.0003692299,0.00025525258,0.0006685688],"category_scores_gemma":[0.0002052406,0.00014768123,0.00012812798,0.00039161724,0.00038763517,0.00016547518,0.00046660207,0.00015650112,0.0002376031],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026010044,0.000050467945,0.9133713,0.000021670066,0.000028126069,0.00077016134,0.0004941486,0.0003928143,0.079935424,0.00033347003,0.00012726213,0.004215014],"study_design_scores_gemma":[0.000014049602,0.00008338452,0.99061066,0.000005399224,0.000020339687,0.00076787424,0.0006572134,0.0017795009,0.0051663034,0.0001223789,0.0007668263,0.0000060875777],"about_ca_topic_score_codex":0.004417405,"about_ca_topic_score_gemma":0.008342821,"teacher_disagreement_score":0.004417405,"about_ca_system_score_codex":0.00034062722,"about_ca_system_score_gemma":0.00009624897,"threshold_uncertainty_score":0.0087834},"labels":[],"label_agreement":null},{"id":"W1963676207","doi":"10.1088/0004-637x/783/2/78","title":"<i>HUBBLE SPACE TELESCOPE</i>/ADVANCED CAMERA FOR SURVEYS CONFIRMATION OF THE DARK SUBSTRUCTURE IN A520","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Dark matter; Centroid; Galaxy; Weak gravitational lensing; Gravitational lens; Mass distribution; Substructure; Galaxy cluster","score_opus":0.0052367107412588125,"score_gpt":0.20839376912458513,"score_spread":0.20315705838332632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963676207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9907352,0.00033290783,0.0008129621,0.00013187865,0.00003529813,0.000020852229,0.0022063006,0.00011890089,0.005605736],"genre_scores_gemma":[0.98995787,0.00010681437,0.0029028528,0.00009424916,0.00004835991,0.000011093256,0.004900218,0.000040208717,0.001938352],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998779,0.0000076338365,0.000010014729,0.000036977523,0.00003556555,0.0000319404],"domain_scores_gemma":[0.99949896,0.000015601829,0.00011581447,0.000049535385,0.00011908129,0.00020099021],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020677509,0.00030284893,0.00017112077,0.0020317477,0.00073268835,0.0004938723,0.00036562732,0.00026153645,0.0026364443],"category_scores_gemma":[0.0002703139,0.00013017301,0.00027263272,0.000784614,0.0002408102,0.00017773344,0.0004560002,0.00018857131,0.0010541887],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041095,0.0001180014,0.84455276,0.0000729835,0.00008004539,0.0019423506,0.00033387702,0.0007650904,0.12918624,0.00094529404,0.0071631526,0.014429224],"study_design_scores_gemma":[0.0000051572724,0.000037435086,0.994418,0.0000074096697,0.000010634308,0.000295319,0.000077719385,0.0007384704,0.0021719295,0.00007099712,0.002159229,0.00000756883],"about_ca_topic_score_codex":0.04393404,"about_ca_topic_score_gemma":0.0564842,"teacher_disagreement_score":0.04393404,"about_ca_system_score_codex":0.00075143593,"about_ca_system_score_gemma":0.00031125525,"threshold_uncertainty_score":0.08735663},"labels":[],"label_agreement":null},{"id":"W1963706634","doi":"10.1088/0004-637x/771/2/113","title":"RADIAL STELLAR PULSATION AND THREE-DIMENSIONAL CONVECTION. II. TWO-DIMENSIONAL CONVECTION IN FULL AMPLITUDE RADIAL PULSATION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Stellar pulsation; Physics; Convection; Amplitude; Light curve; Mechanics; Instability strip; Instability; Coordinate system; Spherical shell; Radial velocity; Classical mechanics; Optics; Geometry; Astrophysics; Shell (structure); Stars; Cepheid variable; Mathematics; Materials science","score_opus":0.009749321783207641,"score_gpt":0.21771010216845907,"score_spread":0.20796078038525143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963706634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.918322,0.00028560267,0.0691002,0.0004217176,0.00009347594,0.00009191419,0.00020382684,0.0005789221,0.010902326],"genre_scores_gemma":[0.9883283,0.00006549523,0.010508284,0.00008549229,0.00001983261,0.000055496253,0.00007916244,0.00010416927,0.0007537657],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985564,0.00004578811,0.0000094110765,0.000018362456,0.00003966654,0.00003108199],"domain_scores_gemma":[0.999595,0.00014768263,0.000074673524,0.00005238768,0.000054572534,0.000075632175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034457367,0.00042403693,0.00038574924,0.00030456187,0.00047245252,0.0007251474,0.0006889054,0.0007297377,0.0009838706],"category_scores_gemma":[0.0015262745,0.00038960367,0.00072304165,0.00029277685,0.00092494057,0.000680472,0.0011393853,0.0007363671,0.0001764885],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007414923,0.000051573028,0.005796322,0.000036667283,0.000030482575,0.00016169247,0.000136292,0.9736665,0.01097724,0.00589096,0.00023087014,0.0029472373],"study_design_scores_gemma":[0.00002949845,0.000017586633,0.0009348812,0.0000027757897,0.0000029045839,0.00002482794,0.000008738389,0.99671006,0.0011214131,0.00083590776,0.00030290068,0.000008517513],"about_ca_topic_score_codex":0.005497577,"about_ca_topic_score_gemma":0.0017482567,"teacher_disagreement_score":0.005497577,"about_ca_system_score_codex":0.00076485705,"about_ca_system_score_gemma":0.0006777579,"threshold_uncertainty_score":0.010931134},"labels":[],"label_agreement":null},{"id":"W1963735602","doi":"10.1086/308446","title":"α Centauri AB","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Opacity; Luminosity; Helium; Stellar evolution; Stars; Stellar mass; Astronomy; Galaxy; Star formation","score_opus":0.00799546705616034,"score_gpt":0.21501888697648733,"score_spread":0.207023419920327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963735602","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34425548,0.0055069583,0.0615299,0.0014087941,0.0014026716,0.00024121653,0.0049818214,0.0038777897,0.57679534],"genre_scores_gemma":[0.9188686,0.0013021729,0.013908938,0.00044462143,0.00009575071,0.00014283271,0.00250649,0.0002330583,0.0624975],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99966383,0.000063718464,0.000019396171,0.0000924097,0.000080064056,0.0000805122],"domain_scores_gemma":[0.9995999,0.000040362527,0.00008092218,0.00011220102,0.0000747194,0.00009191161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004829365,0.0010196961,0.00040312152,0.0019354159,0.0011468885,0.0026948226,0.0010573324,0.0005627107,0.016688295],"category_scores_gemma":[0.0014053287,0.00032982868,0.000606299,0.00096372364,0.00078030943,0.0012445054,0.0012902294,0.00074008876,0.007811822],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001230528,0.00016840069,0.15619662,0.0005292708,0.0003061899,0.0012057002,0.005527702,0.038505122,0.012333882,0.45038718,0.050976798,0.2826326],"study_design_scores_gemma":[0.00014183535,0.00047941846,0.11907463,0.00037203287,0.00020900206,0.0032038286,0.0015739792,0.061603628,0.0041189324,0.1456989,0.6632752,0.00024856537],"about_ca_topic_score_codex":0.010139037,"about_ca_topic_score_gemma":0.004504972,"teacher_disagreement_score":0.016688295,"about_ca_system_score_codex":0.0010277104,"about_ca_system_score_gemma":0.0006278986,"threshold_uncertainty_score":0.055827856},"labels":[],"label_agreement":null},{"id":"W1963758471","doi":"10.1086/498882","title":"Chemical Compositions of Red Giant Stars in Old Large Magellanic Cloud Globular Clusters","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Globular cluster; Physics; Large Magellanic Cloud; Stars; Red giant; Galaxy; Giant star; Red-giant branch; Astronomy","score_opus":0.0057878313006950455,"score_gpt":0.20760099046644104,"score_spread":0.201813159165746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963758471","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962044,0.000063784886,0.000026352172,0.0000042170554,8.921152e-7,0.0000015562209,0.00010133972,0.000004265634,0.000177137],"genre_scores_gemma":[0.99916506,0.000039148053,0.00012322646,0.0000095111345,0.0000026992943,0.00000243618,0.00039190002,0.0000052351243,0.00026075725],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983275,0.000011946183,0.000012992389,0.00005878172,0.00003686923,0.000046692716],"domain_scores_gemma":[0.9994535,0.00005616282,0.00013242524,0.00003810386,0.00013332469,0.00018660568],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021584216,0.00030603382,0.00029712246,0.0022078382,0.00065216265,0.00055620575,0.00045469502,0.0003001344,0.0007356086],"category_scores_gemma":[0.00060633424,0.00023826462,0.00015719266,0.0013124406,0.00040075855,0.00025655865,0.0005281362,0.00014422383,0.00023101651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010087953,0.000019448533,0.979879,0.000012639806,0.000033178523,0.000096377495,0.00045036248,0.0001815409,0.01703181,0.000042696145,0.000059359412,0.0020926918],"study_design_scores_gemma":[0.0000029235773,0.00002257646,0.99836296,0.0000019612103,0.000009324024,0.00006609702,0.00015221516,0.00016988213,0.0009668208,0.000018341427,0.00022354024,0.000003477454],"about_ca_topic_score_codex":0.018830746,"about_ca_topic_score_gemma":0.02742299,"teacher_disagreement_score":0.018830746,"about_ca_system_score_codex":0.0012040943,"about_ca_system_score_gemma":0.00019168737,"threshold_uncertainty_score":0.037442267},"labels":[],"label_agreement":null},{"id":"W1963761446","doi":"10.1088/0004-637x/769/2/108","title":"DISCOVERY OF THE OPTICAL COUNTERPARTS TO FOUR ENERGETIC<i>FERMI</i>MILLISECOND PULSARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":150,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministério da Ciência, Tecnologia e Inovação; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Pulsar; Millisecond pulsar; Physics; Astrophysics; Fermi Gamma-ray Space Telescope; Neutron star; Astronomy; Pulsar planet; X-ray pulsar; Luminosity; Binary pulsar; Galaxy","score_opus":0.009703766820599006,"score_gpt":0.2744891633906275,"score_spread":0.26478539657002853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963761446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986985,0.0001427579,0.0002754871,0.000023569672,0.0000036701094,0.0000021655342,0.00003061,0.000010250445,0.00081301376],"genre_scores_gemma":[0.9989379,0.00010931173,0.0004914018,0.000027490287,0.000012885335,0.0000031150648,0.00015034594,0.0000027657463,0.0002648392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999416,0.0000033019803,0.0000045331794,0.000018284522,0.000011232231,0.000021043708],"domain_scores_gemma":[0.9995597,0.00007382178,0.0002456208,0.00003272237,0.000031407784,0.0000567424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013351151,0.00020942792,0.00012313998,0.0008736882,0.00037191407,0.000667734,0.00019030189,0.00030498262,0.0007696464],"category_scores_gemma":[0.00045602134,0.00013793279,0.0001057893,0.00045981322,0.000337139,0.0002964222,0.0006173989,0.0002442794,0.0001625486],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039258928,0.00006579548,0.80350745,0.000056785604,0.000047848283,0.0020833295,0.00096288417,0.00015348879,0.12960859,0.0008664185,0.00032185408,0.06193304],"study_design_scores_gemma":[0.000012464285,0.0002275941,0.970609,0.000012523095,0.000060104954,0.0039258134,0.00033394733,0.00024440416,0.020175925,0.00044099527,0.003945055,0.000012096753],"about_ca_topic_score_codex":0.0006177356,"about_ca_topic_score_gemma":0.0006781284,"teacher_disagreement_score":0.0008736882,"about_ca_system_score_codex":0.00020828308,"about_ca_system_score_gemma":0.000078852616,"threshold_uncertainty_score":0.0025747418},"labels":[],"label_agreement":null},{"id":"W1963828161","doi":"10.1086/308544","title":"Models for Old, Metal‐poor Stars with Enhanced α‐Element Abundances. I. Evolutionary Tracks and ZAHB Loci; Observational Constraints","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":323,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Stars; Abundance of the chemical elements; Opacity; Red-giant branch; Stellar evolution; Chemical evolution; Helium; Abundance (ecology); Red giant; Horizontal branch; Metallicity; Atomic physics","score_opus":0.019801615277198734,"score_gpt":0.2336172485336107,"score_spread":0.21381563325641198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963828161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92883015,0.00042491916,0.055432606,0.0002719075,0.000024791756,0.00010613298,0.0026756732,0.0002972389,0.011936603],"genre_scores_gemma":[0.96707535,0.00028929024,0.023767812,0.00007931808,0.000029153513,0.00017334345,0.0021560693,0.00009706435,0.006332585],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991393,0.000026991944,0.0000056412778,0.000021581345,0.000011277387,0.000020504896],"domain_scores_gemma":[0.9995747,0.00016829971,0.00008891977,0.000040350733,0.000049356644,0.00007839901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042819802,0.00052649865,0.0005902855,0.0006077801,0.0006496038,0.00087215396,0.0017058224,0.0009584763,0.0023894315],"category_scores_gemma":[0.0010956248,0.00046326022,0.00091375783,0.0005002183,0.0004134883,0.00070054113,0.0005878015,0.00051760365,0.000609956],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011151083,0.000046442445,0.022380356,0.000047103724,0.000044581346,0.00025403372,0.0001610865,0.9611324,0.0016681503,0.011325165,0.00065649714,0.002172563],"study_design_scores_gemma":[0.0001022891,0.000045565565,0.00749592,0.000017094486,0.000034189838,0.000104740786,0.00008551548,0.9831441,0.00036966318,0.0061334004,0.0024507095,0.000016867365],"about_ca_topic_score_codex":0.01650425,"about_ca_topic_score_gemma":0.0246107,"teacher_disagreement_score":0.01650425,"about_ca_system_score_codex":0.0012561657,"about_ca_system_score_gemma":0.0005490729,"threshold_uncertainty_score":0.03281641},"labels":[],"label_agreement":null},{"id":"W1963985428","doi":"10.1086/500388","title":"NLTE Strontium and Barium in Metal‐poor Red Giant Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Strontium; Metallicity; Physics; Astrophysics; Stars; Opacity; Barium; Thermodynamic equilibrium; Line (geometry); Giant star; Abundance (ecology); Chemistry; Thermodynamics; Geometry","score_opus":0.007026642778164579,"score_gpt":0.20405338163821232,"score_spread":0.19702673886004773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963985428","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.978798,0.00033303155,0.011582575,0.00039432273,0.000029620185,0.000012367435,0.00032641564,0.00024095546,0.008282675],"genre_scores_gemma":[0.9974291,0.000121429395,0.0012602587,0.000034258737,0.000015306676,0.00000925876,0.00010841443,0.00004454762,0.0009774283],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999248,0.000025825482,0.000003945763,0.000019472322,0.000013956099,0.000011989582],"domain_scores_gemma":[0.99985254,0.00004582803,0.000032295535,0.000015735157,0.000022989672,0.000030586274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017777598,0.00044632514,0.00033573993,0.0003198375,0.00043253705,0.0007489927,0.0011103906,0.00074328267,0.0012674786],"category_scores_gemma":[0.0005688691,0.00023064962,0.0005777604,0.00030387857,0.00048682073,0.00066556496,0.00069887843,0.00034935147,0.00023769237],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001400822,0.000049673086,0.020497177,0.00005636164,0.000078444216,0.00035252093,0.0001892016,0.9524359,0.007413585,0.015580572,0.0005478971,0.0026584198],"study_design_scores_gemma":[0.00006928814,0.00007383024,0.006489853,0.000009878696,0.000040959414,0.000095557916,0.000067863795,0.9850086,0.0011365621,0.005125098,0.0018642925,0.000018248526],"about_ca_topic_score_codex":0.018629493,"about_ca_topic_score_gemma":0.0089222295,"teacher_disagreement_score":0.018629493,"about_ca_system_score_codex":0.00069488736,"about_ca_system_score_gemma":0.00038157954,"threshold_uncertainty_score":0.03704214},"labels":[],"label_agreement":null},{"id":"W1963987515","doi":"10.1088/0004-637x/721/2/1748","title":"TOWARD UNDERSTANDING THE ENVIRONMENT OF R MONOCEROTIS FROM HIGH-RESOLUTION NEAR-INFRARED POLARIMETRIC OBSERVATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Radiative transfer; Position angle; Polarization (electrochemistry); Circumstellar envelope; Infrared; Polarimetry; Conical surface; Perpendicular; Millimeter; Offset (computer science); Stars; Optics; Scattering; Galaxy","score_opus":0.038353669714786535,"score_gpt":0.22682094057985708,"score_spread":0.18846727086507054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1963987515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9780424,0.00042382645,0.01820312,0.00011099763,0.0000035756298,0.000017867924,0.0002642573,0.0001983052,0.0027355433],"genre_scores_gemma":[0.99452245,0.00015472245,0.0049305935,0.000019823086,0.0000063940565,0.0000033480853,0.00017877517,0.000023478102,0.00016029093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999294,0.000019706455,0.0000022368567,0.000019211515,0.000013235197,0.00001614712],"domain_scores_gemma":[0.9997824,0.00005323376,0.00008074414,0.00003071991,0.000019009069,0.000034034503],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023492273,0.0003070125,0.00034767596,0.0003911479,0.00044449305,0.00074403925,0.00034466913,0.0003940178,0.00058041356],"category_scores_gemma":[0.0006001419,0.0003845378,0.00029199716,0.00040529243,0.0003817336,0.0005921879,0.0005602946,0.00036228256,0.00027846338],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047634167,0.00018380515,0.5643553,0.0002766021,0.00014621642,0.0014486959,0.00089879456,0.20396759,0.18405932,0.0060900715,0.00091991236,0.037177287],"study_design_scores_gemma":[0.000029655892,0.0001284775,0.5391017,0.000020517837,0.000057409947,0.0007265223,0.00048402566,0.44235453,0.010543408,0.0027626993,0.0037337511,0.000057267942],"about_ca_topic_score_codex":0.02083679,"about_ca_topic_score_gemma":0.02794542,"teacher_disagreement_score":0.02083679,"about_ca_system_score_codex":0.00075518433,"about_ca_system_score_gemma":0.0004548422,"threshold_uncertainty_score":0.04143101},"labels":[],"label_agreement":null},{"id":"W1964026845","doi":"10.1088/0004-637x/785/2/137","title":"TRANSIENT SPIRALS AS SUPERPOSED INSTABILITIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Scattering; Amplitude; Stars; Astrophysics; RADIUS; Spiral galaxy; Angular momentum; Dissipative system; Transient (computer programming); Position (finance); Instability; Spiral (railway); Mechanics; Classical mechanics; Optics","score_opus":0.010029344875119556,"score_gpt":0.22970472014762958,"score_spread":0.21967537527251002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964026845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98062176,0.000128195,0.014295569,0.00013011583,0.000018246934,0.000021142443,0.00006233912,0.0002364052,0.004486244],"genre_scores_gemma":[0.99808514,0.000038383172,0.0013918823,0.00001542047,0.0000043404766,0.000009551731,0.000036719695,0.00002629256,0.00039243727],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980456,0.000037434176,0.00001285848,0.00003948629,0.000052178308,0.00005343591],"domain_scores_gemma":[0.9991202,0.00023653737,0.0001680335,0.00014220524,0.00010781387,0.00022525481],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002876842,0.00027796126,0.00029757095,0.00050977396,0.00034099666,0.0012367188,0.0005669346,0.0005130938,0.0027711778],"category_scores_gemma":[0.0021485342,0.00021665847,0.0004972419,0.00033678612,0.0006692848,0.0008831591,0.0011816855,0.00050650287,0.0002250592],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012862488,0.0003162681,0.13383657,0.0003479321,0.00039750914,0.0038928378,0.0055539906,0.6304129,0.090542935,0.09006777,0.0027044918,0.04064055],"study_design_scores_gemma":[0.0001403195,0.00028247928,0.023351736,0.000050890878,0.00009870197,0.00051048707,0.0005898029,0.94209766,0.0076790517,0.020578528,0.0045658727,0.00005450269],"about_ca_topic_score_codex":0.0019910622,"about_ca_topic_score_gemma":0.0014886786,"teacher_disagreement_score":0.0027711778,"about_ca_system_score_codex":0.000583628,"about_ca_system_score_gemma":0.00045813163,"threshold_uncertainty_score":0.009270489},"labels":[],"label_agreement":null},{"id":"W1964062366","doi":"10.1088/0004-637x/736/2/159","title":"REAL-TIME DETECTION AND RAPID MULTIWAVELENGTH FOLLOW-UP OBSERVATIONS OF A HIGHLY SUBLUMINOUS TYPE II-P SUPERNOVA FROM THE PALOMAR TRANSIENT FACTORY SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Observatory; Supernova; Transient (computer programming); Telescope; Sky; Astrophysics; Schmidt camera; Astronomy; Luminosity; Galaxy","score_opus":0.037597354108349995,"score_gpt":0.21879703748889295,"score_spread":0.18119968338054296,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964062366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99594146,0.00017789216,0.0007819607,0.0001426284,0.000017381875,0.000030935844,0.001662131,0.00007628569,0.0011693196],"genre_scores_gemma":[0.99419844,0.000139826,0.001270402,0.00007153059,0.00003316854,0.000028772454,0.0035335922,0.000022113773,0.0007020501],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985385,0.000021201882,0.000008448805,0.000038764112,0.00003864585,0.000039037495],"domain_scores_gemma":[0.9990534,0.00009780064,0.00033593,0.000119681215,0.00012812497,0.00026492996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005997342,0.0002592225,0.00026644155,0.0011677175,0.00028129292,0.0004519256,0.0003780356,0.00031292654,0.00084064336],"category_scores_gemma":[0.00061185734,0.00023213949,0.00026008798,0.0005515524,0.00012488953,0.00026366685,0.0010175655,0.0003655928,0.00042588642],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051786535,0.0001002572,0.9593343,0.00003295089,0.000113847826,0.0010301869,0.0002658162,0.0002104396,0.024103453,0.00010334958,0.0016134696,0.012574141],"study_design_scores_gemma":[0.00001167247,0.000052944368,0.99798113,0.0000024798335,0.000023956063,0.00038131073,0.000065879714,0.00018786814,0.0005189291,0.000019711135,0.00074974843,0.000004412184],"about_ca_topic_score_codex":0.0038846852,"about_ca_topic_score_gemma":0.0078112343,"teacher_disagreement_score":0.0038846852,"about_ca_system_score_codex":0.00022487581,"about_ca_system_score_gemma":0.00026977222,"threshold_uncertainty_score":0.0077241063},"labels":[],"label_agreement":null},{"id":"W1964120515","doi":"10.1088/0004-637x/744/1/58","title":"MULTIPLE STELLAR POPULATIONS IN 47 Tucanae","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":257,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Ministero dell’Istruzione, dell’Università e della Ricerca; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Subgiant; Horizontal branch; Photometry (optics); Red-giant branch; Globular cluster; Stars; Stellar population; Red giant; Blue straggler; Stellar evolution","score_opus":0.04333835082030139,"score_gpt":0.2583890253201166,"score_spread":0.21505067449981521,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964120515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990565,0.000051967854,0.00013052512,0.00001393474,0.000001621831,0.000003268206,0.000106727864,0.000011204889,0.0006241649],"genre_scores_gemma":[0.9989266,0.000028151731,0.0003493502,0.000007447524,0.0000030840042,0.000004611532,0.0004078098,0.000007887547,0.00026508007],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980944,0.000007729298,0.000004344775,0.00006636744,0.00004417897,0.00006792924],"domain_scores_gemma":[0.99975973,0.000023288405,0.00005117143,0.00002282103,0.00006355791,0.000079565674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017799444,0.00026777448,0.0004982128,0.0018461567,0.0019094488,0.001347402,0.00084673637,0.0006404916,0.0015529874],"category_scores_gemma":[0.00056117674,0.00025730973,0.00031970642,0.0015207618,0.00065037503,0.00044681382,0.0007104381,0.00032877887,0.00020488321],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032199328,0.00009923337,0.91691464,0.00003888852,0.00020871812,0.00044963017,0.0011701027,0.016727647,0.034270108,0.0020145914,0.00066745223,0.027117088],"study_design_scores_gemma":[0.000019946143,0.000042486325,0.97446966,0.000009384577,0.00004278901,0.00022188542,0.0006892076,0.019365465,0.002712078,0.00042342025,0.00197732,0.000026220936],"about_ca_topic_score_codex":0.23158906,"about_ca_topic_score_gemma":0.2148135,"teacher_disagreement_score":0.23158906,"about_ca_system_score_codex":0.0035944872,"about_ca_system_score_gemma":0.0011202231,"threshold_uncertainty_score":0.46048218},"labels":[],"label_agreement":null},{"id":"W1964126099","doi":"10.1088/0004-637x/700/1/183","title":"INFRARED SPECTROGRAPH SPECTROSCOPY AND MULTI-WAVELENGTH STUDY OF LUMINOUS STAR-FORMING GALAXIES AT<i>z</i>≃ 1.9","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Victoria; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Spectrograph; Active galactic nucleus; Luminous infrared galaxy; Spectral energy distribution; Photometry (optics); Infrared; Luminosity; Redshift","score_opus":0.008863124085247637,"score_gpt":0.22578665879589133,"score_spread":0.21692353471064368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964126099","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987269,0.00005586764,0.0003017027,0.000009007195,7.866122e-7,0.0000060894836,0.00026749753,0.000016235586,0.00061589736],"genre_scores_gemma":[0.99667007,0.000067026034,0.0011419947,0.000015120454,0.000007023568,0.000010584487,0.0015209529,0.000008340797,0.0005589191],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998498,0.0000142496965,0.000008068689,0.000041598443,0.000035319026,0.00005097307],"domain_scores_gemma":[0.99951065,0.000056495668,0.00020056844,0.000052058458,0.00006398782,0.00011623286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018348252,0.00022315898,0.00019558087,0.002163207,0.0002634741,0.00039822108,0.00026361932,0.00020889923,0.00091182144],"category_scores_gemma":[0.00033381936,0.00012623252,0.0002832934,0.0013010987,0.00014719901,0.00021783584,0.00028170325,0.00018926193,0.00038469196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059617116,0.00009355425,0.9783313,0.000010576299,0.000029206052,0.00008618375,0.00017264165,0.0002719728,0.013060429,0.0001666319,0.00012954033,0.00758829],"study_design_scores_gemma":[0.0000010600296,0.000022308946,0.99883336,7.027025e-7,0.000005707352,0.000052608513,0.00004283422,0.0002085429,0.0006036263,0.000018375005,0.00020976423,0.00000108554],"about_ca_topic_score_codex":0.0041505815,"about_ca_topic_score_gemma":0.0064631375,"teacher_disagreement_score":0.0041505815,"about_ca_system_score_codex":0.0002527999,"about_ca_system_score_gemma":0.000106381274,"threshold_uncertainty_score":0.0082527995},"labels":[],"label_agreement":null},{"id":"W1964157789","doi":"10.1086/432497","title":"Measuring the Cosmic Evolution of Dark Energy with Baryonic Oscillations in the Galaxy Power Spectrum","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Dark energy; Baryon acoustic oscillations; Redshift; Cosmic microwave background; Baryon; Spectral density; Galaxy; Oscillation (cell signaling); Matter power spectrum; Universe","score_opus":0.0063453253233276274,"score_gpt":0.18730657205724174,"score_spread":0.18096124673391412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964157789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8959484,0.000096471565,0.099216424,0.00009899194,0.000013422143,0.000022333159,0.00032430858,0.00031618058,0.003963445],"genre_scores_gemma":[0.9844727,0.000037152484,0.01507297,0.00001130547,0.00000494431,0.000010928177,0.00014563484,0.000027187743,0.00021722945],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996928,0.00011453119,0.00001239134,0.000081229715,0.00007651828,0.000022622946],"domain_scores_gemma":[0.99804235,0.000972146,0.00040147078,0.00038433264,0.00010046284,0.000099367724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00095576874,0.00028615398,0.00021544535,0.0007791485,0.00025070706,0.0007747488,0.0005798352,0.00039588302,0.0008843072],"category_scores_gemma":[0.0059182993,0.0003259519,0.0003098864,0.0007164099,0.000429703,0.00071369164,0.0005316059,0.00036518907,0.0001875292],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000211518,0.00014618172,0.3147288,0.00005860804,0.00027340895,0.00017557504,0.00023332954,0.60270077,0.01861774,0.032966334,0.00045708872,0.029430654],"study_design_scores_gemma":[0.000015253137,0.000044857974,0.0564629,0.0000126917475,0.000027611302,0.00007196436,0.00001922927,0.92621213,0.0072875735,0.009059888,0.00074947224,0.00003630282],"about_ca_topic_score_codex":0.006294401,"about_ca_topic_score_gemma":0.0061375042,"teacher_disagreement_score":0.006294401,"about_ca_system_score_codex":0.0006349446,"about_ca_system_score_gemma":0.00030466006,"threshold_uncertainty_score":0.012515545},"labels":[],"label_agreement":null},{"id":"W1964486795","doi":"10.1088/0004-637x/726/1/47","title":"DISCOVERY OF TIDAL TAILS AROUND THE DISTANT GLOBULAR CLUSTER PALOMAR 14","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Ministerio de Ciencia e Innovación; Centre National de la Recherche Scientifique; Agence Nationale de la Recherche","keywords":"Globular cluster; Physics; Astrophysics; Milky Way; Astronomy; Stars; Orbit (dynamics); Star cluster; Galaxy; Cluster (spacecraft); Halo","score_opus":0.006584663884938956,"score_gpt":0.21534440279337452,"score_spread":0.20875973890843558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964486795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990231,0.000023679095,0.00017161718,0.000017357701,0.000002013462,0.0000035361124,0.000048148424,0.0000139692675,0.0006966158],"genre_scores_gemma":[0.99905723,0.000016752761,0.00039024797,0.000010896293,0.00000405396,0.0000037678171,0.00025386,0.0000042946313,0.0002588758],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999329,0.000004146068,0.000002321583,0.000021738786,0.000020106949,0.000018861101],"domain_scores_gemma":[0.99956363,0.000045611894,0.00013553919,0.000058342954,0.00006665962,0.00013036367],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012132257,0.00018749917,0.00020576731,0.0006869393,0.0006082692,0.00046269488,0.0004285527,0.00026110094,0.0008982119],"category_scores_gemma":[0.0005251494,0.00018028688,0.00012447282,0.00045517788,0.0004560259,0.00020043767,0.0009878648,0.00026458246,0.00022116321],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027253604,0.000063193715,0.90266526,0.000042884498,0.00007191664,0.0026684585,0.0012539162,0.000528002,0.075288855,0.0005396808,0.00053179613,0.016073516],"study_design_scores_gemma":[0.00001406972,0.000107129155,0.99288094,0.0000064429755,0.000022640184,0.001162038,0.0002901948,0.0008206279,0.0030046795,0.00023125007,0.0014469688,0.0000130019935],"about_ca_topic_score_codex":0.0034368834,"about_ca_topic_score_gemma":0.0067913346,"teacher_disagreement_score":0.0034368834,"about_ca_system_score_codex":0.00032796615,"about_ca_system_score_gemma":0.00026482172,"threshold_uncertainty_score":0.0068337917},"labels":[],"label_agreement":null},{"id":"W1964516851","doi":"10.1086/378978","title":"Carbon Isotope Ratio in<sup>12</sup>CO/<sup>13</sup>CO toward Local Molecular Clouds with Near‐Infrared High‐Resolution Spectroscopy of Vibrational Transition Bands","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Université de Montréal","funders":"","keywords":"Physics; Infrared; Spectroscopy; Carbon monoxide; Extinction (optical mineralogy); Isotopologue; Radiative transfer; Astrophysics; Molecular cloud; Analytical Chemistry (journal); Atomic physics; Spectral line; Astronomy; Chemistry; Stars","score_opus":0.006132193118799951,"score_gpt":0.21540209749324446,"score_spread":0.2092699043744445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964516851","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991548,0.00007269316,0.00014161522,0.0000057380144,0.0000010417225,0.0000014144393,0.00011385931,0.000011407346,0.0004974261],"genre_scores_gemma":[0.9993861,0.000028512144,0.00017822658,0.00000612757,0.0000018653596,0.0000025104316,0.00022311213,0.0000044847966,0.00016903064],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999341,0.0000034539312,0.000002471056,0.000018032508,0.000022827948,0.000019071336],"domain_scores_gemma":[0.99987423,0.00001195346,0.000046704048,0.000009921511,0.000035901325,0.000021307113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007842002,0.00019409208,0.0000944138,0.0004347511,0.00023279867,0.00027874997,0.00024714874,0.00015208378,0.0010748334],"category_scores_gemma":[0.00014713909,0.000091088674,0.000102292826,0.00030523192,0.00018259733,0.0001729722,0.00014283007,0.00015427024,0.00021280334],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005453206,0.00003071894,0.46294048,0.000044688677,0.00007482489,0.00021218753,0.00012075659,0.00054710155,0.5275043,0.000088402616,0.00023258157,0.0076586027],"study_design_scores_gemma":[0.000004887686,0.000053830398,0.95640844,0.000003079158,0.00002580046,0.00020282858,0.000083826206,0.0008634539,0.04200263,0.000022213535,0.00032309917,0.000005851976],"about_ca_topic_score_codex":0.007937646,"about_ca_topic_score_gemma":0.016000692,"teacher_disagreement_score":0.007937646,"about_ca_system_score_codex":0.00029924721,"about_ca_system_score_gemma":0.00008457353,"threshold_uncertainty_score":0.015782893},"labels":[],"label_agreement":null},{"id":"W1964655925","doi":"10.1088/0004-637x/779/2/98","title":"TWO SUPERLUMINOUS SUPERNOVAE FROM THE EARLY UNIVERSE DISCOVERED BY THE SUPERNOVA LEGACY SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Defence Research and Development Canada; University of Toronto","funders":"","keywords":"Supernova; Physics; Astrophysics; Redshift; Dark energy; Galaxy; Universe; Astronomy; Cosmology","score_opus":0.013144408386013063,"score_gpt":0.22125928280899956,"score_spread":0.2081148744229865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964655925","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99740005,0.0001291991,0.00018119198,0.000020965437,0.000008414433,0.000010244345,0.0014337075,0.000026953472,0.00078926596],"genre_scores_gemma":[0.9877772,0.0002321359,0.0010013272,0.00004295115,0.000023980534,0.000013838782,0.009873222,0.00001817863,0.0010171899],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997975,0.000021555776,0.000014968247,0.000035357723,0.00007067489,0.000059857284],"domain_scores_gemma":[0.99894565,0.00011963704,0.00039813673,0.0000888794,0.00008818454,0.00035957148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003455143,0.00053981395,0.0003144862,0.0029480807,0.00044458357,0.0005246306,0.00036717436,0.0003673832,0.0015905595],"category_scores_gemma":[0.00057007547,0.00022804787,0.00038849917,0.0010948833,0.000309667,0.00031950136,0.0012141487,0.00038846472,0.0002668768],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008007929,0.0002849473,0.9681616,0.000044213735,0.00015354421,0.0009888137,0.0002906955,0.00040043806,0.014597146,0.0003549617,0.0008434815,0.013079394],"study_design_scores_gemma":[0.000021395384,0.00012535672,0.99392575,0.0000048383163,0.00002188472,0.0011366949,0.000089091845,0.0003516796,0.0019243896,0.00009585892,0.0022934827,0.000009575618],"about_ca_topic_score_codex":0.0052333474,"about_ca_topic_score_gemma":0.021390786,"teacher_disagreement_score":0.0052333474,"about_ca_system_score_codex":0.00028200555,"about_ca_system_score_gemma":0.00018300921,"threshold_uncertainty_score":0.010405779},"labels":[],"label_agreement":null},{"id":"W1964675623","doi":"10.1088/0004-637x/731/2/94","title":"SOLAR-LIKE OSCILLATIONS AND ACTIVITY IN PROCYON: A COMPARISON OF THE 2007<i>MOST</i>AND GROUND-BASED RADIAL VELOCITY CAMPAIGNS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Saint Mary's University","funders":"","keywords":"Physics; Amplitude; Photometry (optics); Astrophysics; Radial velocity; Oscillation (cell signaling); Scaling; Spectral density; Stars; Astronomy; Optics; Statistics; Geometry","score_opus":0.02503336046945746,"score_gpt":0.24055841012823836,"score_spread":0.21552504965878092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964675623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99707854,0.00015625179,0.00007158143,0.000026073323,0.0000035904661,0.000003090606,0.001539609,0.000025780451,0.0010955004],"genre_scores_gemma":[0.9922712,0.00018638237,0.00054063695,0.000028809887,0.000014932425,0.000007163911,0.006653332,0.000025751484,0.00027189092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982965,0.00001672665,0.000010620068,0.00007388412,0.000033064898,0.00003606997],"domain_scores_gemma":[0.9991352,0.00009827315,0.0003345906,0.00011795568,0.00016083148,0.00015323101],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027286,0.00024374499,0.00026292002,0.0014545392,0.00027395273,0.0005449618,0.0002266093,0.00021952264,0.0006773104],"category_scores_gemma":[0.0006023343,0.00014335237,0.00023313385,0.0010536887,0.00024282942,0.00032335077,0.0007528444,0.00021509458,0.0002106855],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029129128,0.00004042634,0.97511214,0.00008456494,0.00012427916,0.00015813657,0.0004849056,0.00059001084,0.007631901,0.00014782943,0.0011813261,0.014153099],"study_design_scores_gemma":[0.0000021934077,0.000019058612,0.99878293,0.0000061187056,0.000009219834,0.000060762475,0.00010186189,0.00012940874,0.00042262254,0.0000082295755,0.00045475308,0.0000029326611],"about_ca_topic_score_codex":0.013792557,"about_ca_topic_score_gemma":0.045527797,"teacher_disagreement_score":0.013792557,"about_ca_system_score_codex":0.00035824685,"about_ca_system_score_gemma":0.00020161648,"threshold_uncertainty_score":0.027424514},"labels":[],"label_agreement":null},{"id":"W1964702173","doi":"10.1086/309465","title":"Embedded, Self‐Gravitating Equilibria in Sheetlike and Filamentary Molecular Clouds","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Western University","funders":"","keywords":"Molecular cloud; Physics; Astrophysics; Materials science","score_opus":0.005144766035155156,"score_gpt":0.231578465791386,"score_spread":0.22643369975623084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964702173","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99364823,0.00014758272,0.0030374113,0.00010304289,0.000012526119,0.000021924478,0.000063358835,0.000048477643,0.0029175042],"genre_scores_gemma":[0.9972229,0.000083504914,0.002098964,0.000018276489,0.000011627585,0.00001631748,0.00006234714,0.000012774801,0.0004732148],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999069,0.000027859081,0.0000059736512,0.000010598082,0.00001815306,0.000030524938],"domain_scores_gemma":[0.9993806,0.00027251994,0.00015780596,0.000023197443,0.000057577952,0.000108245054],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031942126,0.000400146,0.00039351836,0.00075439055,0.0007595331,0.0013698622,0.00088098773,0.00084799994,0.0012802436],"category_scores_gemma":[0.0023706125,0.00031264144,0.00033183052,0.00060036615,0.0012528975,0.00066470064,0.00089946185,0.00045222207,0.000100806144],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023134422,0.00017475871,0.01350275,0.000085623156,0.0000730092,0.00073910464,0.00042317758,0.9540649,0.0037856128,0.023495633,0.0005310603,0.0028930649],"study_design_scores_gemma":[0.00010547786,0.000073843854,0.00267484,0.00001541217,0.000017218064,0.000068322675,0.00016854254,0.99227446,0.00044025376,0.00385042,0.00029851336,0.000012751939],"about_ca_topic_score_codex":0.01073409,"about_ca_topic_score_gemma":0.005534519,"teacher_disagreement_score":0.01073409,"about_ca_system_score_codex":0.0010917053,"about_ca_system_score_gemma":0.0005378049,"threshold_uncertainty_score":0.021343231},"labels":[],"label_agreement":null},{"id":"W1964786144","doi":"10.1088/0004-637x/791/1/43","title":"COMPARISON OF PRESTELLAR CORE ELONGATIONS AND LARGE-SCALE MOLECULAR CLOUD STRUCTURES IN THE LUPUS I REGION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Protein filament; Physics; Molecular cloud; Astrophysics; Parsec; Core (optical fiber); Magnetic field; Orientation (vector space); Scale (ratio); Bent molecular geometry; Geometry; Galaxy; Optics; Materials science; Stars","score_opus":0.014872251863386789,"score_gpt":0.27535261891340473,"score_spread":0.2604803670500179,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964786144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994055,0.000035682737,0.00006075213,0.0000041760195,3.0601853e-7,8.14249e-7,0.00006968788,0.0000035068624,0.00041950264],"genre_scores_gemma":[0.9997389,0.0000175828,0.000044623328,0.0000031706065,0.0000013124321,6.0752456e-7,0.00014181953,0.0000024715466,0.00004957436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991465,0.000008303709,0.0000068265113,0.00003254132,0.00001162259,0.000026085],"domain_scores_gemma":[0.9994429,0.00010630371,0.00022846313,0.0000512027,0.000038933686,0.00013209009],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015333545,0.00010116736,0.00011223442,0.0007605271,0.00013730605,0.00043700144,0.00017619978,0.00017506303,0.00085853407],"category_scores_gemma":[0.0005695234,0.000101230275,0.00017817394,0.00032736233,0.0002232854,0.00029026877,0.0002623261,0.00011407821,0.00016482889],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036343842,0.00003461119,0.93465656,0.000022496472,0.000077583114,0.00022030645,0.00027788192,0.001149334,0.05608004,0.00033195782,0.00008938964,0.0066964696],"study_design_scores_gemma":[0.0000030007448,0.000021544583,0.99842775,0.0000014137604,0.0000062943705,0.00007419202,0.00005430645,0.00038176798,0.0009159728,0.000041497435,0.000070615635,0.000001775761],"about_ca_topic_score_codex":0.0022502,"about_ca_topic_score_gemma":0.0021634365,"teacher_disagreement_score":0.0022502,"about_ca_system_score_codex":0.0002946345,"about_ca_system_score_gemma":0.00008378836,"threshold_uncertainty_score":0.0044742227},"labels":[],"label_agreement":null},{"id":"W1964821336","doi":"10.1086/427748","title":"The Millisecond Pulsars in NGC 6760","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Millisecond pulsar; Globular cluster; Physics; Pulsar; Astrophysics; Astronomy; Binary pulsar; Cluster (spacecraft); Interstellar medium; Galaxy","score_opus":0.008925220725945843,"score_gpt":0.3059783982516108,"score_spread":0.29705317752566496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1964821336","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984875,0.00013961479,0.000042892134,0.000012273131,0.000004190815,0.0000017537672,0.00022588507,0.0000094546185,0.001076451],"genre_scores_gemma":[0.997834,0.00018660132,0.00012134855,0.000019441357,0.0000061629344,0.000003467732,0.0013106557,0.0000044366757,0.0005137743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987996,0.000006182878,0.0000057839993,0.000021033748,0.000036321293,0.000050567458],"domain_scores_gemma":[0.9997578,0.000023859873,0.0000730165,0.000021855953,0.000032729546,0.00009058851],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011362061,0.00018573012,0.00018041155,0.0012661435,0.00041798063,0.00033973536,0.00012226433,0.00015943385,0.0011078565],"category_scores_gemma":[0.00026036162,0.00009140261,0.00012752027,0.0011022436,0.0001891591,0.0001479036,0.0005590392,0.00014247396,0.00034922178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002996149,0.000077528646,0.9398717,0.000051893152,0.00006031146,0.0009785736,0.00086047413,0.00058603875,0.037557952,0.00045803565,0.0010482289,0.018149596],"study_design_scores_gemma":[0.0000048515744,0.000021505492,0.997903,0.00000419185,0.000008923734,0.00014867516,0.00012479721,0.0001363987,0.00050923554,0.000057850266,0.0010771092,0.0000034670988],"about_ca_topic_score_codex":0.026812773,"about_ca_topic_score_gemma":0.042746477,"teacher_disagreement_score":0.026812773,"about_ca_system_score_codex":0.00031330742,"about_ca_system_score_gemma":0.00016183627,"threshold_uncertainty_score":0.053313375},"labels":[],"label_agreement":null},{"id":"W1965021087","doi":"10.1086/591120","title":"The Role of the Radial Orbit Instability in Dark Matter Halo Formation and Structure","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Instability; Halo; Astrophysics; Dark matter; Velocity dispersion; Isotropy; Perturbation (astronomy); Dark matter halo; RADIUS; Mechanics; Astronomy; Galaxy; Optics","score_opus":0.0037957424098562513,"score_gpt":0.17990901541913037,"score_spread":0.17611327300927412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965021087","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868775,0.0006180566,0.006891821,0.00035693907,0.000022605953,0.000022069406,0.000052790747,0.00013480114,0.005023424],"genre_scores_gemma":[0.99884254,0.0001297808,0.0007916488,0.000022189564,0.0000054499087,0.000004604048,0.000017897533,0.000019583455,0.00016638271],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985707,0.00004621173,0.000008270749,0.00001926498,0.000030256548,0.00003897832],"domain_scores_gemma":[0.99948883,0.00011977369,0.00015315767,0.000045012515,0.00004598965,0.00014724227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054407294,0.0006119375,0.00041285815,0.00044439753,0.0009363676,0.00113321,0.0005031792,0.0005847914,0.001136031],"category_scores_gemma":[0.0021081686,0.00031190043,0.0004798099,0.0002003488,0.0009552663,0.0011217763,0.0011400774,0.00053910667,0.00017691105],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052862195,0.00017310768,0.08890777,0.0001968206,0.00022754488,0.00080607185,0.00070078566,0.78079504,0.08104186,0.033191793,0.0008183015,0.012612271],"study_design_scores_gemma":[0.000104724735,0.00015471809,0.029453905,0.000028582925,0.000036684265,0.000145444,0.00015985253,0.9466879,0.007970671,0.0143428985,0.00083518133,0.00007952926],"about_ca_topic_score_codex":0.008722691,"about_ca_topic_score_gemma":0.0043839826,"teacher_disagreement_score":0.008722691,"about_ca_system_score_codex":0.001158056,"about_ca_system_score_gemma":0.0009865937,"threshold_uncertainty_score":0.01734382},"labels":[],"label_agreement":null},{"id":"W1965152300","doi":"10.1088/0004-637x/777/1/1","title":"WITNESSING THE DIFFERENTIAL EVOLUTION OF DISK GALAXIES IN LUMINOSITY AND SIZE VIA GRAVITATIONAL LENSING","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Galaxy formation and evolution; Luminous infrared galaxy; Luminosity; Redshift; Population; Elliptical galaxy; Gravitational lens","score_opus":0.005475600219524386,"score_gpt":0.198923249027978,"score_spread":0.1934476488084536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965152300","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999134,0.00008020651,0.00022356678,0.000015293761,5.590182e-7,0.0000013496636,0.00010695297,0.000010355917,0.00042768585],"genre_scores_gemma":[0.99959856,0.000035617413,0.0001435668,0.0000054551474,0.0000021481953,7.8147076e-7,0.00011283161,0.000002974756,0.00009809359],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998783,0.000016215845,0.0000052423197,0.000037497502,0.000024809877,0.000037935533],"domain_scores_gemma":[0.99889624,0.00027498882,0.00043993737,0.00009198629,0.00009520503,0.00020151523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027991005,0.00018440456,0.00018266647,0.0013393788,0.00020287126,0.0004973936,0.00022707021,0.00020682496,0.0005291006],"category_scores_gemma":[0.0013122689,0.00016207655,0.0001646517,0.0008736968,0.00034616233,0.00043791512,0.0004780493,0.00021012439,0.00013190255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054894248,0.000014925453,0.9726413,0.000012451301,0.000038129732,0.0001317485,0.00030402179,0.0007285555,0.019380735,0.00059341505,0.000100851066,0.0059989695],"study_design_scores_gemma":[0.0000011247533,0.000012343256,0.997982,9.546595e-7,0.0000056359545,0.00006124551,0.00004634474,0.0008740959,0.00077455153,0.00011175203,0.00012725707,0.000002584017],"about_ca_topic_score_codex":0.008246009,"about_ca_topic_score_gemma":0.008459163,"teacher_disagreement_score":0.008246009,"about_ca_system_score_codex":0.00049850217,"about_ca_system_score_gemma":0.00012728568,"threshold_uncertainty_score":0.016395986},"labels":[],"label_agreement":null},{"id":"W1965166130","doi":"10.1088/0004-637x/726/2/64","title":"PARAMETERIZING AND MEASURING DARK ENERGY TRAJECTORIES FROM LATE INFLATONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Quintessence; Dark energy; Redshift; Cosmic microwave background; Astrophysics; Parameter space; Cosmology; Galaxy; Quantum mechanics; Statistics","score_opus":0.00829346942306517,"score_gpt":0.21709390028255665,"score_spread":0.2088004308594915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965166130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95096344,0.000045613007,0.047853284,0.000031656677,0.0000025885754,0.000012193148,0.00014428562,0.000085422915,0.00086146727],"genre_scores_gemma":[0.9894777,0.00005891633,0.009974816,0.000004632727,0.0000014863834,0.000014985935,0.00026506648,0.0000229036,0.00017939947],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99987817,0.000053247648,0.000006590999,0.00003214392,0.000016254487,0.00001364476],"domain_scores_gemma":[0.99884856,0.0005868895,0.00023162208,0.00017252627,0.000062068066,0.00009838748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008481652,0.00037801522,0.00023978311,0.00058035937,0.0003086816,0.0007863029,0.0004400346,0.0003839887,0.0005796476],"category_scores_gemma":[0.0042682607,0.00039696743,0.000353187,0.00048476172,0.0005898432,0.0008735295,0.00054928026,0.00059635524,0.00011864036],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015277913,0.000044373915,0.08822514,0.000029242337,0.000070980896,0.000087529756,0.00019962579,0.87107414,0.007838003,0.023027616,0.00011558227,0.009134847],"study_design_scores_gemma":[0.0000062150552,0.00002685471,0.0125122,0.000010078154,0.000010712344,0.00003432412,0.00003256701,0.97669625,0.0033400233,0.007068395,0.0002407143,0.000021693026],"about_ca_topic_score_codex":0.008797181,"about_ca_topic_score_gemma":0.0079481285,"teacher_disagreement_score":0.008797181,"about_ca_system_score_codex":0.0008992365,"about_ca_system_score_gemma":0.0005769014,"threshold_uncertainty_score":0.017491937},"labels":[],"label_agreement":null},{"id":"W1965166314","doi":"10.1088/0004-637x/799/2/194","title":"AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: NEAR-INFRARED MORPHOLOGIES AND STELLAR SIZES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Surface brightness; Galaxy; Chandra Deep Field South; RADIUS; Star formation; Brightness; Astronomy","score_opus":0.02152498100055098,"score_gpt":0.24031785143095463,"score_spread":0.21879287043040366,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965166314","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911341,0.00067164894,0.00047695357,0.00019549229,0.000025639196,0.000028139011,0.0050931163,0.000102096565,0.0022729307],"genre_scores_gemma":[0.9900864,0.00037931412,0.0012305868,0.00020707438,0.000072471004,0.000024547566,0.006303393,0.00003382054,0.0016624334],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976784,0.000021211383,0.000013033827,0.000071039445,0.00006692506,0.000059987862],"domain_scores_gemma":[0.99827635,0.00014233604,0.00053347694,0.0002078476,0.0003638996,0.00047606928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004371008,0.00032117864,0.00038266345,0.0028589363,0.0004624982,0.0006595571,0.00039430073,0.00024213793,0.0015989898],"category_scores_gemma":[0.0006975494,0.00027381536,0.00034349397,0.0022227743,0.00025862805,0.00058964785,0.00085855566,0.00037339618,0.00056976016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015138458,0.00008798762,0.95523256,0.000056048582,0.00011596481,0.0001261951,0.00041720824,0.00013523105,0.015979644,0.00031804116,0.0063052373,0.02107449],"study_design_scores_gemma":[0.00000504475,0.000012592053,0.9975667,0.0000055216324,0.000018330538,0.00010639415,0.000088816836,0.000120312856,0.00037658826,0.00002929804,0.0016643186,0.00000617744],"about_ca_topic_score_codex":0.0118577685,"about_ca_topic_score_gemma":0.038863346,"teacher_disagreement_score":0.0118577685,"about_ca_system_score_codex":0.00040601593,"about_ca_system_score_gemma":0.0005705177,"threshold_uncertainty_score":0.023577511},"labels":[],"label_agreement":null},{"id":"W1965265700","doi":"10.1088/0004-637x/749/1/94","title":"ERRATUM: “CLOSE COMPANIONS TO YOUNG STARS. I. A LARGE SPECTROSCOPIC SURVEY IN CHAMAELEON I AND TAURUS-AURIGA” (2012, ApJ, 745, 119)","year":2012,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"History and Developments in Astronomy","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Stars; Astrophysics; Astronomy","score_opus":0.014213191711001895,"score_gpt":0.2526094163251047,"score_spread":0.23839622461410281,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965265700","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00077158667,0.0023201406,0.00023510495,0.028703397,0.9565463,0.000028331971,0.0025094596,0.0002638576,0.008621799],"genre_scores_gemma":[0.02003322,0.016000124,0.0033315192,0.08357107,0.30158108,0.00016817165,0.013783838,0.001501211,0.5600297],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99873966,0.00012247646,0.0003118807,0.00018284861,0.0005218717,0.00012127801],"domain_scores_gemma":[0.9928929,0.0012878533,0.0005455595,0.00047278404,0.0043137297,0.00048712286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012010656,0.0021432766,0.0014648052,0.0034853085,0.0036861328,0.0023587772,0.0019187588,0.003249432,0.046401557],"category_scores_gemma":[0.013868898,0.0008411185,0.0011644308,0.002256156,0.0009618826,0.0018246659,0.0015299801,0.0043280115,0.03370447],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000035179546,0.000009663798,0.0002074779,0.000069928596,0.0000063311436,0.00026619734,0.000019334962,0.00002123676,0.00006241861,0.00016529894,0.99400157,0.005135409],"study_design_scores_gemma":[0.00003713263,0.000042077907,0.0051094443,0.0003482956,0.000044116452,0.0008985369,0.00015441918,0.00008802854,0.00039138814,0.00048478995,0.992361,0.000040919702],"about_ca_topic_score_codex":0.02975133,"about_ca_topic_score_gemma":0.04527462,"teacher_disagreement_score":0.046401557,"about_ca_system_score_codex":0.0021870534,"about_ca_system_score_gemma":0.002894256,"threshold_uncertainty_score":0.15522867},"labels":[],"label_agreement":null},{"id":"W1965356258","doi":"10.1088/0004-637x/777/2/105","title":"MOCK OBSERVATIONS OF BLUE STRAGGLERS IN GLOBULAR CLUSTER MODELS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Blue straggler; Globular cluster; Milky Way; Cluster (spacecraft); Stellar evolution; Star cluster; Stellar collision","score_opus":0.022554437626870736,"score_gpt":0.2211071470881703,"score_spread":0.19855270946129958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965356258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983576,0.000015838665,0.0011847508,0.000016562899,0.0000015171636,0.000009563345,0.0001228502,0.00004506348,0.00024618482],"genre_scores_gemma":[0.9984769,0.000011816604,0.001060716,0.000008560593,0.0000012734456,0.000010246568,0.00028516582,0.000010914283,0.00013432461],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99960476,0.00015407427,0.000017496113,0.000107283035,0.00005346213,0.00006287417],"domain_scores_gemma":[0.9974964,0.0010803042,0.0003663529,0.00042700034,0.00029641378,0.00033338618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010438801,0.00031958576,0.0003245429,0.0007194559,0.00046461725,0.00066323794,0.0009470671,0.0006725509,0.0005121461],"category_scores_gemma":[0.0041172276,0.00030588856,0.00038053206,0.0005894958,0.0006301311,0.00050205475,0.0005927642,0.0004155837,0.00010905632],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009216511,0.00022894061,0.25688413,0.000055135813,0.00014199178,0.00031795187,0.00084034336,0.715871,0.0115611795,0.0071192244,0.00095080584,0.0051077106],"study_design_scores_gemma":[0.00006472342,0.00017581975,0.053621147,0.0000110517185,0.00002878712,0.00008830265,0.00011323416,0.9393166,0.003572036,0.0021458894,0.00082343793,0.000039044404],"about_ca_topic_score_codex":0.015388061,"about_ca_topic_score_gemma":0.015590964,"teacher_disagreement_score":0.015388061,"about_ca_system_score_codex":0.0020571337,"about_ca_system_score_gemma":0.0004287151,"threshold_uncertainty_score":0.030597031},"labels":[],"label_agreement":null},{"id":"W1965451881","doi":"10.1086/592263","title":"Electrodynamics of Magnetars. III. Pair Creation Processes in an Ultrastrong Magnetic Field and Particle Heating in a Dynamic Magnetosphere","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Magnetosphere; Magnetic field; Positronium; Magnetar; Pair production; Atomic physics; Field line; Computational physics; Quantum electrodynamics; Electron; Positron; Nuclear physics; Quantum mechanics","score_opus":0.006731114321815664,"score_gpt":0.2785177759201828,"score_spread":0.2717866615983671,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965451881","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8283866,0.0063021793,0.07930277,0.00231122,0.00032247405,0.000067855035,0.00012014781,0.00020682748,0.08297991],"genre_scores_gemma":[0.9898235,0.0006240109,0.0018013616,0.00012421241,0.000095593205,0.000029154502,0.000024488258,0.000024824292,0.0074527166],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999287,0.000017137947,0.000002066008,0.000008845853,0.00001532034,0.000027913677],"domain_scores_gemma":[0.9999089,0.00002190546,0.00002542981,0.000010739743,0.0000125546185,0.000020475854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013995572,0.00024803326,0.00026280974,0.0003018274,0.000463011,0.0007545872,0.00039547207,0.00052142056,0.0019962576],"category_scores_gemma":[0.0004215118,0.0001610458,0.0002543627,0.00018629698,0.0009951182,0.0008461859,0.00084916677,0.0003179844,0.00035314992],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023952816,0.0000918599,0.007709463,0.00011370901,0.000067690366,0.0013413441,0.0008284996,0.16058818,0.041297182,0.7652344,0.003993976,0.018494248],"study_design_scores_gemma":[0.00016395685,0.00042432922,0.028592529,0.000051341438,0.00003766019,0.0014352943,0.00082729734,0.53821903,0.006879436,0.40466475,0.018596236,0.00010819177],"about_ca_topic_score_codex":0.0009132935,"about_ca_topic_score_gemma":0.00045023614,"teacher_disagreement_score":0.0019962576,"about_ca_system_score_codex":0.00052397716,"about_ca_system_score_gemma":0.00016172489,"threshold_uncertainty_score":0.0066781044},"labels":[],"label_agreement":null},{"id":"W1965508181","doi":"10.1086/422575","title":"Enhanced Extra Mixing in Low‐Mass Red Giants: Lithium Production and Thermal Stability","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Angular momentum; Stars; Red-giant branch; Mixing (physics); Metallicity; Stellar evolution; Luminosity; Rotation (mathematics); Angular velocity; Astronomy; Classical mechanics; Galaxy","score_opus":0.011061167316470659,"score_gpt":0.21869718516633715,"score_spread":0.2076360178498665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965508181","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987348,0.00019498463,0.0005150917,0.000033520384,0.0000013842445,6.427519e-7,0.000024852221,0.000012651371,0.00048208493],"genre_scores_gemma":[0.9997212,0.000037558246,0.00010773593,0.000007390186,0.0000018185924,6.104595e-7,0.000020422965,0.0000013228914,0.00010202362],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999745,0.0000027951196,0.0000016717248,0.000009370558,0.0000039535453,0.000007762592],"domain_scores_gemma":[0.9998259,0.00002664416,0.00009312301,0.000014741579,0.0000076607075,0.000032006246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000089324116,0.00017039526,0.00017243947,0.0002427026,0.0002043909,0.0005881705,0.00019434025,0.00030126792,0.0006986983],"category_scores_gemma":[0.0003006857,0.000090268506,0.00014069877,0.00019506537,0.00035096265,0.00033133547,0.00055254024,0.00016256333,0.00019655468],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066741294,0.00004682847,0.4470588,0.0001439851,0.00008576362,0.0015879327,0.00051336066,0.008422789,0.52091944,0.009024185,0.00035379734,0.011175635],"study_design_scores_gemma":[0.00009342469,0.00033473628,0.7341456,0.000037326223,0.00020334823,0.005421464,0.000471038,0.10618024,0.13352446,0.015909676,0.0036157314,0.000062967854],"about_ca_topic_score_codex":0.00076127285,"about_ca_topic_score_gemma":0.00057236676,"teacher_disagreement_score":0.00076127285,"about_ca_system_score_codex":0.0003489075,"about_ca_system_score_gemma":0.00009152288,"threshold_uncertainty_score":0.0025315285},"labels":[],"label_agreement":null},{"id":"W1965509586","doi":"10.1086/342228","title":"Weak Lensing Study of Galaxy Biasing","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"","score_opus":0.017628129941934544,"score_gpt":0.22319966213892167,"score_spread":0.20557153219698712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965509586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92764145,0.007859312,0.026313279,0.004526517,0.0002175937,0.00001623426,0.00014377813,0.00013461853,0.03314721],"genre_scores_gemma":[0.9924739,0.0011074775,0.0015215,0.00014029318,0.00028198623,0.000004166012,0.00004091292,0.000018659093,0.004411169],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9998282,0.000053092415,0.0000062506892,0.000045358633,0.0000343707,0.000032772703],"domain_scores_gemma":[0.99628276,0.001970105,0.00047100367,0.000294508,0.0006108415,0.00037086706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001293432,0.00029199186,0.00038670655,0.0009296741,0.0004340109,0.000974585,0.00048414455,0.00031576306,0.0026893497],"category_scores_gemma":[0.006697246,0.00016511268,0.00021362484,0.00068841677,0.00088991894,0.0010283074,0.00057276,0.0006256248,0.00018720691],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036075866,0.000081821534,0.10194415,0.00042175956,0.0002643586,0.0008529464,0.0008592197,0.010575964,0.02793632,0.76641417,0.0060918885,0.084196575],"study_design_scores_gemma":[0.00011489431,0.00016482275,0.16815785,0.0000756733,0.00020076658,0.0012370073,0.00074695697,0.11539361,0.007939894,0.69013596,0.01574628,0.000086273394],"about_ca_topic_score_codex":0.0019607814,"about_ca_topic_score_gemma":0.0011384767,"teacher_disagreement_score":0.0026893497,"about_ca_system_score_codex":0.0005577807,"about_ca_system_score_gemma":0.00026340102,"threshold_uncertainty_score":0.008996785},"labels":[],"label_agreement":null},{"id":"W1965571089","doi":"10.1086/424660","title":"Ultraviolet Absorption in Amorphous Carbons: Polycyclic Aromatic Hydrocarbons and the 2175 Å Extinction Feature","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Carbon Nanotubes in Composites","field":"Materials Science","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Coronene; Polycyclic aromatic hydrocarbon; Amorphous solid; Amorphous carbon; Absorption (acoustics); Absorption spectroscopy; Extinction (optical mineralogy); Ultraviolet; Astrochemistry; Physics; Photochemistry; Analytical Chemistry (journal); Interstellar medium; Astrophysics; Molecule; Chemistry; Astrobiology; Galaxy; Organic chemistry; Optics","score_opus":0.0053289508852152265,"score_gpt":0.21512960257508815,"score_spread":0.2098006516898729,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965571089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99693394,0.00039915205,0.00079980725,0.000014934189,0.000003487777,0.0000024806425,0.000028046987,0.000022489368,0.0017957587],"genre_scores_gemma":[0.9989968,0.00008343419,0.00043824673,0.0000063608422,0.0000015736354,0.0000015105458,0.000040959032,0.0000027648177,0.00042835998],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999542,0.0000039080883,0.0000013866235,0.000008490446,0.000023121413,0.000008777614],"domain_scores_gemma":[0.9999281,0.00001960846,0.000023127714,0.0000060136417,0.000013107334,0.000010032093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000047961697,0.00011398068,0.000055738987,0.00031666626,0.0002633902,0.00016300663,0.00013140003,0.00018642137,0.00086470955],"category_scores_gemma":[0.00010158739,0.00006667728,0.000064165164,0.00020976826,0.00025660463,0.00011921736,0.00008154926,0.0001709114,0.00009928253],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002945112,0.00001007551,0.0013571521,0.00002063002,0.000003889578,0.000092637994,0.00002883849,0.00010728327,0.9963491,0.00024558415,0.000028789631,0.0017264278],"study_design_scores_gemma":[0.0000046201626,0.00013159693,0.021094615,0.0000052009486,0.000008520665,0.00041221915,0.000050134302,0.00072395365,0.9762999,0.00017721868,0.0010884318,0.0000035658568],"about_ca_topic_score_codex":0.00048070395,"about_ca_topic_score_gemma":0.0007877399,"teacher_disagreement_score":0.00086470955,"about_ca_system_score_codex":0.00014121691,"about_ca_system_score_gemma":0.00006343762,"threshold_uncertainty_score":0.0028927326},"labels":[],"label_agreement":null},{"id":"W1965642093","doi":"10.1086/587164","title":"Glimm’s Method for Relativistic Hydrodynamics","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Classification of discontinuities; Piecewise; Mathematics; Riemann problem; Mathematical analysis; Applied mathematics; Riemann hypothesis","score_opus":0.015617670848069901,"score_gpt":0.2596612738905469,"score_spread":0.244043603042477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965642093","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011262645,0.0002903097,0.9934029,0.00014294498,0.00018874352,0.000066518645,0.00021495491,0.0013421166,0.0032253233],"genre_scores_gemma":[0.023732468,0.0003300873,0.968506,0.00015072268,0.00008184309,0.00043011812,0.00038373133,0.001071029,0.0053139552],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99943537,0.0001964231,0.000037505066,0.00005955937,0.000226799,0.000044299617],"domain_scores_gemma":[0.9987153,0.0005217122,0.00008648864,0.00026890193,0.00035197238,0.000055794848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015629587,0.0008057975,0.00086105085,0.0011787934,0.00055780297,0.0009478561,0.0020097184,0.0013479315,0.009921222],"category_scores_gemma":[0.0043518655,0.0005591588,0.0012996285,0.0011981055,0.0008203599,0.0009909063,0.0015139941,0.0021107863,0.004607203],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017484707,0.00009023884,0.0015815245,0.00061100273,0.0001690205,0.00035724425,0.00024166444,0.29082742,0.007204623,0.32377988,0.047193352,0.32776925],"study_design_scores_gemma":[0.00005466689,0.000040192142,0.0003685329,0.000047131463,0.000020925754,0.00020534259,0.000022058244,0.88718414,0.002681662,0.046181522,0.06314344,0.00005037567],"about_ca_topic_score_codex":0.0031802184,"about_ca_topic_score_gemma":0.0028681282,"teacher_disagreement_score":0.009921222,"about_ca_system_score_codex":0.00067659427,"about_ca_system_score_gemma":0.002040028,"threshold_uncertainty_score":0.033189774},"labels":[],"label_agreement":null},{"id":"W1965692720","doi":"10.1086/309221","title":"Resolving the Jeans Mass in Hydrodynamic Simulations of Hierarchical Clustering","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Western University","funders":"","keywords":"Substructure; Physics; Baryon; Dark matter; Halo; Cosmology; Resolution (logic); Structure formation; Component (thermodynamics); Astrophysics; Offset (computer science); Statistical physics; Galaxy; Thermodynamics","score_opus":0.006371911964088853,"score_gpt":0.215946925239841,"score_spread":0.20957501327575215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965692720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98904055,0.00014699518,0.007318184,0.0003742635,0.000027804255,0.000033605887,0.00009171324,0.00019142828,0.002775392],"genre_scores_gemma":[0.9956909,0.00007303591,0.003620609,0.000065475644,0.000017723438,0.000027802373,0.00008024478,0.0000408347,0.00038349643],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996147,0.00014733584,0.000018975781,0.000037779544,0.000066517336,0.0001146969],"domain_scores_gemma":[0.99684024,0.0018297784,0.000381906,0.00015840262,0.00028406622,0.000505621],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015398602,0.00059121026,0.0006704211,0.00090210704,0.0011326504,0.0011110589,0.0010770479,0.001324753,0.00072821975],"category_scores_gemma":[0.00792898,0.0006083339,0.00055445085,0.0007819404,0.001443123,0.0010518228,0.00126164,0.0009560188,0.000113184076],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008376255,0.00006429626,0.0066474294,0.000019543575,0.000035004243,0.00008435842,0.0001404239,0.98633945,0.0009765751,0.004179049,0.0002584671,0.0011717252],"study_design_scores_gemma":[0.000027951883,0.000014404872,0.00052527775,0.0000027122876,0.000005179615,0.0000051257584,0.000019072364,0.9983329,0.00017880532,0.0007995788,0.000081640996,0.000007333821],"about_ca_topic_score_codex":0.05510521,"about_ca_topic_score_gemma":0.025172902,"teacher_disagreement_score":0.05510521,"about_ca_system_score_codex":0.0025851303,"about_ca_system_score_gemma":0.0014107354,"threshold_uncertainty_score":0.109568894},"labels":[],"label_agreement":null},{"id":"W1965697993","doi":"10.1086/504371","title":"The Distribution of Ortho–H<sub>2</sub>D<sup>+</sup>(1<sub>1,0</sub>–1<sub>1,1</sub>) in L1544: Tracing the Deuteration Factory in Prestellar Cores","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Deuterium; Physics; RADIUS; Atomic physics; Astrochemistry; Hydrogen; Order (exchange); Chemistry; Analytical Chemistry (journal); Astrophysics; Interstellar medium","score_opus":0.007187080621752726,"score_gpt":0.2108372875003494,"score_spread":0.2036502068785967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965697993","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994228,0.000021773103,0.00007881151,0.0000068471086,4.3787634e-7,0.0000010236355,0.00009357438,0.000006402013,0.00036830257],"genre_scores_gemma":[0.99943584,0.00001705701,0.00010155608,0.0000061250475,0.0000014491903,0.000002443482,0.0002000785,0.0000036811723,0.00023177131],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997187,0.0000019020788,0.0000014825134,0.000010951649,0.000004250643,0.000009512825],"domain_scores_gemma":[0.99991846,0.000010091566,0.00002678648,0.000005458069,0.000012822886,0.000026309273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005683096,0.00013951257,0.00011939097,0.0004846691,0.00016978708,0.0002460247,0.0002613704,0.00021175468,0.0014706161],"category_scores_gemma":[0.00010641974,0.00014970887,0.00009598271,0.00016447219,0.00021816259,0.00016056772,0.00021668844,0.00014423634,0.00025285606],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040253907,0.00006491016,0.451403,0.000028203147,0.00003589749,0.0003354734,0.0001649138,0.0017495959,0.53809136,0.000561277,0.0001980188,0.006964714],"study_design_scores_gemma":[0.00000925754,0.00005177642,0.9764415,0.0000028096938,0.000010671126,0.00016347932,0.00014282533,0.002798405,0.019865898,0.00013094707,0.00037515876,0.00000723719],"about_ca_topic_score_codex":0.0052246093,"about_ca_topic_score_gemma":0.005230809,"teacher_disagreement_score":0.0052246093,"about_ca_system_score_codex":0.00048037988,"about_ca_system_score_gemma":0.000080236154,"threshold_uncertainty_score":0.010388434},"labels":[],"label_agreement":null},{"id":"W1965699302","doi":"10.1086/595746","title":"An Improved Method for Using Mg <scp>ii</scp> to Estimate Black Hole Masses in Active Galactic Nuclei","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Active galactic nucleus; Astrophysics; Redshift; Luminosity; Sky; Black hole (networking); Line (geometry); Quasar; Accretion (finance); Galaxy; Geometry","score_opus":0.017070913139952335,"score_gpt":0.2915315925665275,"score_spread":0.27446067942657515,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965699302","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.06330416,0.00040622908,0.9172968,0.0001569683,0.00012320501,0.00020357016,0.0038222135,0.009259391,0.0054275],"genre_scores_gemma":[0.3008366,0.00020942479,0.6898035,0.00016471883,0.00015595176,0.00030189686,0.0043355483,0.0007926096,0.0033996874],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9990289,0.00011423725,0.00007913239,0.00028636865,0.0004393367,0.000052113915],"domain_scores_gemma":[0.9981621,0.00030063593,0.00036216923,0.0005247077,0.0005747071,0.000075671705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012601856,0.0006386306,0.0004938921,0.0038293155,0.0005969247,0.0012560609,0.0011527676,0.00047479203,0.0024515942],"category_scores_gemma":[0.005292224,0.00039410137,0.00055979233,0.0019102477,0.00029454345,0.00076048507,0.0010052171,0.00072855083,0.0019724306],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002821436,0.00012491185,0.16589956,0.00023266094,0.0004847235,0.0004355006,0.00040052758,0.020320442,0.089789666,0.010059018,0.013636938,0.69833386],"study_design_scores_gemma":[0.00014496277,0.00019589816,0.29028824,0.00008320051,0.00019464058,0.0015994118,0.00015469486,0.49386865,0.09352945,0.023948602,0.0957226,0.00026976023],"about_ca_topic_score_codex":0.007893396,"about_ca_topic_score_gemma":0.0080331955,"teacher_disagreement_score":0.007893396,"about_ca_system_score_codex":0.00042408888,"about_ca_system_score_gemma":0.0005676375,"threshold_uncertainty_score":0.015694857},"labels":[],"label_agreement":null},{"id":"W1965708197","doi":"10.1086/368070","title":"Very Long Baseline Interferometry Imaging of the RS Canum Venaticorum Binary Star System HR 5110","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Subgiant; Very-long-baseline interferometry; Stars; Binary star; Full width at half maximum; Halo; Brightness; Astronomy; Galaxy; Globular cluster; Optics","score_opus":0.007344034718505576,"score_gpt":0.20886340502170134,"score_spread":0.20151937030319575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965708197","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99316275,0.00012858043,0.00021765275,0.00004393242,0.000009001697,0.0000075615035,0.00042781088,0.000040803177,0.0059618033],"genre_scores_gemma":[0.99739695,0.00005455358,0.0005898623,0.000024755482,0.000009853268,0.0000067239484,0.0011413812,0.0000063946927,0.00076956616],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99985003,0.000010408801,0.0000046427303,0.000036425103,0.000038879592,0.00005956033],"domain_scores_gemma":[0.99983513,0.000014862297,0.0000356111,0.000021644817,0.00003385007,0.00005887303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014623886,0.00014698302,0.00017374763,0.0009539588,0.00032507954,0.00036654974,0.00036750038,0.00034034922,0.0015948846],"category_scores_gemma":[0.0003183144,0.00015827495,0.000093000555,0.00042917492,0.00014157852,0.00015924471,0.00033872842,0.00020580931,0.00040646188],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012186425,0.00042304877,0.34763855,0.00012208601,0.00011731228,0.0016239451,0.00055955246,0.0031342595,0.57589126,0.001386699,0.008068436,0.059816215],"study_design_scores_gemma":[0.000024048102,0.00009245636,0.99020994,0.000009145649,0.000017474305,0.0003942309,0.00008222878,0.0020108672,0.0046434836,0.00005841736,0.002447615,0.000010064476],"about_ca_topic_score_codex":0.017335849,"about_ca_topic_score_gemma":0.0471826,"teacher_disagreement_score":0.017335849,"about_ca_system_score_codex":0.000956766,"about_ca_system_score_gemma":0.0002493024,"threshold_uncertainty_score":0.034469903},"labels":[],"label_agreement":null},{"id":"W1965712495","doi":"10.1086/500422","title":"Nonlinear Decline‐Rate Dependence and Intrinsic Variation of Type Ia Supernova Luminosities","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Supernova; Luminosity; Light curve; Line (geometry); Type (biology); Statistics; Mathematics; Geometry; Galaxy","score_opus":0.008825560901170705,"score_gpt":0.23029410164142908,"score_spread":0.22146854074025837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965712495","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989489,0.000081389786,0.0060818545,0.000016737544,0.0000037884818,0.000009211811,0.0005629693,0.00021417357,0.003540842],"genre_scores_gemma":[0.995915,0.00005308674,0.0013055227,0.000008633571,0.000003927609,0.000012026202,0.0016196418,0.00009445629,0.000987676],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955696,0.000092188835,0.000036104248,0.00014227553,0.00012499288,0.00004749821],"domain_scores_gemma":[0.99634594,0.001385665,0.00071569404,0.00090729684,0.0005406852,0.00010477423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001199043,0.00035075712,0.00027391408,0.00087886397,0.00016238533,0.0008184431,0.0004977536,0.0002501176,0.0015564064],"category_scores_gemma":[0.0054431222,0.00036894015,0.0006896027,0.0006606564,0.00026444878,0.0004125499,0.0005708715,0.0004736283,0.00086119806],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027135952,0.000064005275,0.8923979,0.000089742796,0.00027261025,0.00007851774,0.00031580095,0.028196814,0.05316441,0.0010422987,0.0004375897,0.023668986],"study_design_scores_gemma":[0.0000070033516,0.00007510616,0.9441048,0.000010816405,0.000044772893,0.00020101425,0.000041365376,0.04498837,0.009149144,0.00041326336,0.0009463108,0.000018047338],"about_ca_topic_score_codex":0.0028392165,"about_ca_topic_score_gemma":0.003138187,"teacher_disagreement_score":0.0028392165,"about_ca_system_score_codex":0.00044824317,"about_ca_system_score_gemma":0.00019560287,"threshold_uncertainty_score":0.0063411593},"labels":[],"label_agreement":null},{"id":"W1965784688","doi":"10.1088/0004-637x/765/2/117","title":"X-RAY GROUPS OF GALAXIES IN THE AEGIS DEEP AND WIDE FIELDS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"University of Pittsburgh; Japan Society for the Promotion of Science; University of California, Santa Cruz; Ministry of Education, Culture, Sports, Science and Technology; National Science Foundation","keywords":"Physics; Astrophysics; Velocity dispersion; Virial theorem; Redshift; Virial mass; Galaxy; RADIUS; Galaxy group; Astronomy; Galaxy cluster","score_opus":0.005524181411574483,"score_gpt":0.1940746363059275,"score_spread":0.18855045489435301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965784688","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947647,0.00014670336,0.0001104897,0.000022706101,0.0000020995453,0.000008676842,0.003672687,0.000014560244,0.0012572915],"genre_scores_gemma":[0.98668075,0.00022886248,0.00075550383,0.000022642696,0.000009976312,0.00001664055,0.011147401,0.00001075469,0.0011273721],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982774,0.000015584099,0.000015343254,0.000059919235,0.000031325286,0.000050008326],"domain_scores_gemma":[0.9994387,0.00006130046,0.00023696007,0.00006748881,0.000053592445,0.0001419462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031440318,0.00029855987,0.00022066043,0.0038709515,0.00025857627,0.00059594895,0.0001529495,0.0001487094,0.0026260978],"category_scores_gemma":[0.00061834056,0.00011048046,0.00020966667,0.0017369617,0.00019100303,0.00045764472,0.0009689407,0.00017239197,0.00044650005],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009907304,0.000027767192,0.9843791,0.00001878978,0.000058419715,0.00008815815,0.00027201587,0.0003428261,0.0030771217,0.0003386174,0.0005513564,0.010746762],"study_design_scores_gemma":[0.0000037176521,0.000012850431,0.99868804,0.0000040815044,0.000008445564,0.000040343133,0.000114170056,0.00017534923,0.00014167275,0.00008213634,0.0007271661,0.000002045252],"about_ca_topic_score_codex":0.011140635,"about_ca_topic_score_gemma":0.013048347,"teacher_disagreement_score":0.011140635,"about_ca_system_score_codex":0.00034727211,"about_ca_system_score_gemma":0.00016924058,"threshold_uncertainty_score":0.02215159},"labels":[],"label_agreement":null},{"id":"W1965861082","doi":"10.1086/312791","title":"[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of Molecular Hydrogen in Translucent Interstellar Clouds: The Line of Sight toward HD 73882","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Mean kinetic temperature; Interstellar cloud; Physics; Astrophysics; Line-of-sight; Molecular cloud; Line (geometry); Interstellar medium; Ultraviolet; Hydrogen; Excitation; Excitation temperature; Molecule; Rotational temperature; Absorption (acoustics); Astrochemistry; Atomic physics; Spectral line; Emission spectrum; Astronomy; Stars; Optics; Galaxy","score_opus":0.01983554197946576,"score_gpt":0.23949737524619624,"score_spread":0.21966183326673047,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965861082","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.05397235,0.010517619,0.0053911377,0.011362651,0.035986077,0.00072029233,0.08326906,0.0040131006,0.7947676],"genre_scores_gemma":[0.09652981,0.009308767,0.005374402,0.0048184604,0.010453304,0.00025872496,0.05191846,0.000968422,0.82036966],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9999399,0.0000033479748,0.0000039643464,0.000015397583,0.000018561488,0.000018805646],"domain_scores_gemma":[0.9997776,0.000035762572,0.00005371548,0.00001676497,0.000062198604,0.000053857413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001241363,0.00078752975,0.0005103211,0.001391983,0.000626935,0.0008365111,0.0007537356,0.00072287326,0.24769327],"category_scores_gemma":[0.00023647715,0.00023721943,0.00052947394,0.0020253467,0.000280409,0.0009934045,0.00043723956,0.0006563594,0.059193663],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006480222,0.000120983445,0.0037101891,0.0005036436,0.00005478223,0.0009181824,0.000045806155,0.00048474903,0.014755909,0.002162733,0.8979931,0.07860181],"study_design_scores_gemma":[0.0001025105,0.0001713107,0.071540244,0.00016752431,0.00003399019,0.00067694305,0.00018203557,0.0002661084,0.0044616945,0.0014301667,0.920939,0.000028438408],"about_ca_topic_score_codex":0.008447924,"about_ca_topic_score_gemma":0.014636748,"teacher_disagreement_score":0.24769327,"about_ca_system_score_codex":0.00033416325,"about_ca_system_score_gemma":0.00023633176,"threshold_uncertainty_score":0.82861656},"labels":[],"label_agreement":null},{"id":"W1965980682","doi":"10.1088/0004-637x/746/1/4","title":"MODELING EXTRAGALACTIC FOREGROUNDS AND SECONDARIES FOR UNBIASED ESTIMATION OF COSMOLOGICAL PARAMETERS FROM PRIMARY COSMIC MICROWAVE BACKGROUND ANISOTROPY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cosmic microwave background; Physics; Planck; Astrophysics; Cosmic infrared background; Cosmology; Spectral density; Cosmic background radiation; COSMIC cancer database; Galaxy; Anisotropy; Statistics; Optics","score_opus":0.024252122758741133,"score_gpt":0.26306283644049955,"score_spread":0.2388107136817584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965980682","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2660482,0.00029138412,0.73180276,0.00016365648,0.000015735592,0.000019462686,0.00018638841,0.00029241134,0.0011800135],"genre_scores_gemma":[0.916214,0.0002854516,0.081861414,0.00004260302,0.00003790026,0.00004707134,0.00044431383,0.000104562576,0.00096270523],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99962497,0.00015005186,0.00001525513,0.00008582236,0.00007023573,0.000053701748],"domain_scores_gemma":[0.9988852,0.0005849737,0.00015714877,0.00026952155,0.000054360666,0.00004869551],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011634573,0.00076614745,0.00048826047,0.00078119896,0.00037417893,0.0010088716,0.00083384063,0.00043369085,0.0012908537],"category_scores_gemma":[0.0046154438,0.00053892203,0.00089870795,0.00079514325,0.0006426102,0.00096738274,0.0009828021,0.00067884394,0.00027771253],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021433833,0.00009580695,0.04200073,0.00009815848,0.00030876408,0.00024258504,0.00033909097,0.77319014,0.014586346,0.10967223,0.0005991345,0.05865278],"study_design_scores_gemma":[0.00001591392,0.000018518587,0.00930771,0.000010598509,0.00004703125,0.00005679494,0.000025688456,0.95513505,0.0020127904,0.03243097,0.00091726135,0.000021771446],"about_ca_topic_score_codex":0.007710066,"about_ca_topic_score_gemma":0.010281384,"teacher_disagreement_score":0.007710066,"about_ca_system_score_codex":0.00075876585,"about_ca_system_score_gemma":0.000960816,"threshold_uncertainty_score":0.015330374},"labels":[],"label_agreement":null},{"id":"W1965989611","doi":"10.1088/0004-637x/714/2/1689","title":"THE DRAO PLANCK DEEP FIELDS: THE POLARIZATION PROPERTIES OF RADIO GALAXIES AT 1.4 GHz","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics; University of Calgary","funders":"","keywords":"Physics; Spectral index; Astrophysics; Polarization (electrochemistry); Source counts; Hubble Deep Field; Sky; Galaxy; Planck; Stokes parameters; Cosmic microwave background; Astronomy; Optics; Redshift; Spectral line; Scattering","score_opus":0.005741383954928304,"score_gpt":0.18439404895474082,"score_spread":0.17865266499981253,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1965989611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9692611,0.0008527459,0.0038940725,0.0002006324,0.000018474866,0.000029096494,0.018125994,0.00032824496,0.00728959],"genre_scores_gemma":[0.9712161,0.00048300158,0.008349839,0.00009492625,0.00007278338,0.00004162394,0.018074429,0.00013904065,0.0015282992],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998385,0.000022473278,0.0000043042164,0.000046273668,0.000036911977,0.000051460935],"domain_scores_gemma":[0.99942434,0.00009356417,0.00021034198,0.00010622907,0.000050679468,0.0001149466],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043618635,0.00035323665,0.0001964477,0.0015509408,0.00024167664,0.00052761944,0.00028192034,0.00014225513,0.0016751759],"category_scores_gemma":[0.0007869948,0.00018507146,0.00017685439,0.0012075843,0.00018100772,0.0005068789,0.00061037496,0.00026142402,0.00047354118],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005128997,0.0001001008,0.7926341,0.0001950507,0.00018549035,0.00033453823,0.0012188728,0.003876763,0.058947712,0.0021179551,0.011661827,0.12821466],"study_design_scores_gemma":[0.000014986645,0.000027126673,0.9882504,0.0000084175035,0.000028483599,0.00014788608,0.00007981295,0.0010502932,0.0021336994,0.0006026549,0.007641061,0.000015222433],"about_ca_topic_score_codex":0.0035099054,"about_ca_topic_score_gemma":0.0035751993,"teacher_disagreement_score":0.0035099054,"about_ca_system_score_codex":0.00027582058,"about_ca_system_score_gemma":0.000110628265,"threshold_uncertainty_score":0.006978929},"labels":[],"label_agreement":null},{"id":"W1966023306","doi":"10.1088/0004-637x/718/2/905","title":"TRACING TURBULENT AMBIPOLAR DIFFUSION IN MOLECULAR CLOUDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Molecular cloud; Turbulence; Magnetic field; Diffusion; Ion; Magnetohydrodynamics; Spectral line","score_opus":0.00540773298151605,"score_gpt":0.22582998018731296,"score_spread":0.2204222472057969,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966023306","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9833241,0.0003457267,0.014384744,0.00013564268,0.000016420834,0.00002060302,0.00012546188,0.000115869836,0.0015313429],"genre_scores_gemma":[0.99661595,0.000091321075,0.00312157,0.000009288572,0.0000057955413,0.000003192021,0.00004021177,0.0000071094514,0.00010546758],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999211,0.000016226317,0.0000037790242,0.00001649115,0.000018438626,0.000023880091],"domain_scores_gemma":[0.9997074,0.00008653222,0.00008831687,0.00002531262,0.000033596032,0.00005885669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025009064,0.0003000969,0.0002403544,0.00093461614,0.00039313722,0.00093929714,0.00042571494,0.0003827032,0.0002831546],"category_scores_gemma":[0.0013192502,0.00025901076,0.00019567937,0.00048587966,0.0005866784,0.0006839497,0.0009715914,0.00034550313,0.00006142854],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012422334,0.00035763747,0.24964117,0.0001720372,0.00021923188,0.0012518893,0.0018369887,0.49844328,0.15356573,0.052200247,0.0012000275,0.039869506],"study_design_scores_gemma":[0.00004008562,0.000050019793,0.020929473,0.000015107038,0.000013132685,0.00008067363,0.00013798849,0.96820015,0.005159731,0.0046349885,0.00070808514,0.000030607294],"about_ca_topic_score_codex":0.010264702,"about_ca_topic_score_gemma":0.0051894076,"teacher_disagreement_score":0.010264702,"about_ca_system_score_codex":0.00069886283,"about_ca_system_score_gemma":0.00029450472,"threshold_uncertainty_score":0.020409882},"labels":[],"label_agreement":null},{"id":"W1966061795","doi":"10.1086/522822","title":"The ACS Fornax Cluster Survey. II. The Central Brightness Profiles of Early-Type Galaxies: A Characteristic Radius on Nuclear Scales and the Transition from Central Luminosity Deficit to Excess","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":131,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Extrapolation; Galaxy; Surface brightness; Surface brightness fluctuation; Astronomy; Fornax Cluster; Luminosity; Luminosity function; RADIUS; Elliptical galaxy; Fundamental plane (elliptical galaxies); Virgo Cluster; Brightest cluster galaxy; Lenticular galaxy; Statistics","score_opus":0.00749687094528425,"score_gpt":0.20602660059286898,"score_spread":0.19852972964758472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966061795","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.46107662,0.0028929003,0.00063701166,0.0034020366,0.0006245111,0.00035355127,0.49001878,0.0011541431,0.03984058],"genre_scores_gemma":[0.65294105,0.0012985078,0.0021099837,0.0006240732,0.00065238884,0.00038897613,0.31196463,0.00033293525,0.029687341],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966025,0.00004329934,0.000028153769,0.000073163894,0.00012331775,0.00007180717],"domain_scores_gemma":[0.99508226,0.00035376355,0.001103342,0.00057779544,0.002011473,0.0008713716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010039685,0.00044703519,0.0005376183,0.0040817787,0.0006035609,0.0008230747,0.0009991679,0.0006778105,0.010731011],"category_scores_gemma":[0.0039613894,0.0004074659,0.0002780845,0.0028444713,0.00043780555,0.001084865,0.00070356095,0.00042066604,0.008648278],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067068165,0.00013306645,0.60897064,0.00028745478,0.000120672215,0.00018050274,0.00025333272,0.0003308513,0.0023533253,0.000694184,0.33894897,0.047056343],"study_design_scores_gemma":[0.000026448532,0.000015517287,0.9856323,0.000010870616,0.000015238938,0.000037531303,0.00004990512,0.00005579341,0.00017520208,0.00007895403,0.013895121,0.0000070440447],"about_ca_topic_score_codex":0.058310244,"about_ca_topic_score_gemma":0.09751566,"teacher_disagreement_score":0.058310244,"about_ca_system_score_codex":0.00070301304,"about_ca_system_score_gemma":0.00059983594,"threshold_uncertainty_score":0.1159417},"labels":[],"label_agreement":null},{"id":"W1966067227","doi":"10.1086/376590","title":"Triggered Star Formation in the W5 H<scp>ii</scp>Region","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Star formation; Stars; Interstellar medium; Young stellar object; Star (game theory); Star cluster; Population; Astronomy; Orion Nebula; H II region; Molecular cloud; Galaxy","score_opus":0.015691547270947934,"score_gpt":0.2327660610058064,"score_spread":0.21707451373485848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966067227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991197,0.00007125277,0.00018938306,0.0000057631223,5.640752e-7,0.000002601277,0.000017629873,0.0000052653986,0.00058772694],"genre_scores_gemma":[0.9996711,0.00003299902,0.00015699398,0.0000052095493,0.0000018872561,0.000001058695,0.000034714092,0.000001027902,0.000095005686],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999466,0.0000062001545,0.0000036197373,0.000014222808,0.000011787636,0.000017549044],"domain_scores_gemma":[0.9998318,0.000019023866,0.0000905085,0.000013388561,0.000015070243,0.000030290832],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001230706,0.000084037376,0.00010004759,0.0002719912,0.0002526447,0.0003562764,0.00013718434,0.00014003328,0.00040935393],"category_scores_gemma":[0.00024615985,0.000107914675,0.00011599862,0.0002142666,0.00019135192,0.00018783665,0.00026756214,0.00008789304,0.00010927764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002917482,0.00008174361,0.8240942,0.000055644123,0.000082247105,0.0028376973,0.0003361699,0.0011807304,0.15133134,0.001330925,0.0003051807,0.018072378],"study_design_scores_gemma":[0.00000923092,0.00016413961,0.9888861,0.000005794052,0.000022154978,0.0015774339,0.00017147043,0.0010436462,0.006997968,0.00025697274,0.0008616103,0.0000034226107],"about_ca_topic_score_codex":0.002273203,"about_ca_topic_score_gemma":0.002474921,"teacher_disagreement_score":0.002273203,"about_ca_system_score_codex":0.00023701235,"about_ca_system_score_gemma":0.0001435284,"threshold_uncertainty_score":0.0045199394},"labels":[],"label_agreement":null},{"id":"W1966106868","doi":"10.1086/518361","title":"Rotation and Activity of Pre–Main‐Sequence Stars","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"","keywords":"Physics; Stars; Astrophysics; T Tauri star; Dynamo; Stellar rotation; Main sequence; myr; Rotation period; Rotation (mathematics); Stellar classification; Spectral line; Astronomy; Sequence (biology); Magnetic field; Geometry","score_opus":0.014246460182010996,"score_gpt":0.2522135795249403,"score_spread":0.23796711934292927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966106868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992694,0.00010247824,0.00004395839,0.000004034262,6.7399935e-7,0.0000018992931,0.00027617268,0.0000036250942,0.00029762875],"genre_scores_gemma":[0.9980902,0.00007825824,0.00010503456,0.000005523561,0.0000075029566,0.0000030074787,0.0014451327,0.0000036061842,0.0002616773],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998523,0.000019907002,0.000013078834,0.00004737682,0.000026799707,0.000040423343],"domain_scores_gemma":[0.9991972,0.00012847991,0.00028781992,0.00008103018,0.000095357136,0.00021016106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020232612,0.00026778263,0.00019765127,0.0017266299,0.0002495928,0.00041009256,0.00013957152,0.00022016633,0.0011834218],"category_scores_gemma":[0.0006027676,0.000099822886,0.00019486496,0.0007814152,0.00020577929,0.00034259216,0.00033747763,0.0001608736,0.0007001911],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000091737485,0.000036149027,0.9911048,0.0000080817845,0.000024214793,0.000050872328,0.00012845873,0.000079423306,0.0044007627,0.000026209766,0.000049731556,0.0039996253],"study_design_scores_gemma":[5.1534585e-7,0.00002587815,0.9995646,5.413189e-7,0.000002243583,0.00006439889,0.0000197679,0.000038850667,0.00016554822,0.000007069951,0.00011003411,6.957252e-7],"about_ca_topic_score_codex":0.0013488934,"about_ca_topic_score_gemma":0.0020760442,"teacher_disagreement_score":0.0017266299,"about_ca_system_score_codex":0.00016106208,"about_ca_system_score_gemma":0.000081650185,"threshold_uncertainty_score":0.0039589405},"labels":[],"label_agreement":null},{"id":"W1966251371","doi":"10.1086/588034","title":"A Cryogenic Liquid‐Mirror Telescope on the Moon to Study the Early Universe","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"ImmerVision (Canada); University of British Columbia; Université Laval","funders":"","keywords":"James Webb Space Telescope; Telescope; Primary mirror; Astronomy; Physics; Sky; Secondary mirror; Astrobiology","score_opus":0.027028742837213536,"score_gpt":0.24364859772823813,"score_spread":0.2166198548910246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966251371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92418444,0.0009680834,0.048907463,0.0010570688,0.00027736623,0.0001450543,0.0005805781,0.0004639706,0.023415966],"genre_scores_gemma":[0.9170498,0.00028699692,0.07410321,0.0002471639,0.000108375294,0.00010027082,0.00078815914,0.00009921024,0.0072167907],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996811,0.000055339195,0.000008987472,0.00006635183,0.00010980331,0.00007845882],"domain_scores_gemma":[0.99932265,0.000082822255,0.000058752237,0.00015067964,0.00019942458,0.00018566837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011038876,0.00023706681,0.0003396476,0.0003412726,0.0005185456,0.00053984846,0.00058902183,0.00040718983,0.0025817978],"category_scores_gemma":[0.0004738182,0.00022016719,0.0004316231,0.00025509225,0.00026573375,0.00068707345,0.00066092005,0.0008856269,0.0008157417],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031694974,0.0001549921,0.015104486,0.00008771873,0.00004279181,0.00029332383,0.0004184457,0.0006885125,0.96128374,0.0032864078,0.0017123411,0.016610308],"study_design_scores_gemma":[0.0003304442,0.0062647187,0.21397421,0.00017272879,0.00034128118,0.0022778828,0.0014166643,0.04006227,0.61705357,0.0028837444,0.11511965,0.000102853664],"about_ca_topic_score_codex":0.0014755988,"about_ca_topic_score_gemma":0.002185124,"teacher_disagreement_score":0.0025817978,"about_ca_system_score_codex":0.0003786119,"about_ca_system_score_gemma":0.0005323262,"threshold_uncertainty_score":0.008637011},"labels":[],"label_agreement":null},{"id":"W1966316634","doi":"10.1086/320093","title":"Intrinsic Shapes of Molecular Cloud Cores","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Western University","funders":"","keywords":"Prolate spheroid; Oblate spheroid; Core (optical fiber); Distribution (mathematics); Molecular cloud; Cloud computing; Physics; Statistical physics; Geometry; Astrophysics; Classical mechanics; Optics; Computer science; Mathematics","score_opus":0.00880579600278136,"score_gpt":0.2067771467300718,"score_spread":0.19797135072729044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966316634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99570036,0.000069310234,0.0022652277,0.000009488699,0.0000013721307,0.000008602061,0.0007264846,0.00005457522,0.0011645523],"genre_scores_gemma":[0.9976363,0.000046238114,0.0011845754,0.000004785941,0.0000033025624,0.0000074176032,0.00094599335,0.0000342188,0.00013716804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997476,0.000030664018,0.000015817424,0.00008360893,0.00006615733,0.000056121728],"domain_scores_gemma":[0.9977259,0.0004291093,0.00069163216,0.0002955828,0.000649768,0.00020802602],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049037056,0.00018691047,0.00021594221,0.0016558361,0.00032109444,0.00077798107,0.0003194182,0.00016191654,0.00097590825],"category_scores_gemma":[0.0032825745,0.00029074016,0.00033517496,0.0008972441,0.00031293786,0.00052354357,0.00048212262,0.00024304322,0.00031030504],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024093603,0.000027489437,0.9091432,0.00006291483,0.00012025124,0.00014299416,0.00032718226,0.014834206,0.054413587,0.0021097949,0.0005203955,0.018057078],"study_design_scores_gemma":[0.00001211089,0.000053909727,0.9346928,0.000009843914,0.00003418391,0.0004068292,0.00013527415,0.047865696,0.014581318,0.0009835,0.0011953156,0.00002911156],"about_ca_topic_score_codex":0.0017903798,"about_ca_topic_score_gemma":0.002643939,"teacher_disagreement_score":0.0017903798,"about_ca_system_score_codex":0.00043809172,"about_ca_system_score_gemma":0.00026730716,"threshold_uncertainty_score":0.003559947},"labels":[],"label_agreement":null},{"id":"W1966324939","doi":"10.1086/381566","title":"Formation of Cool Cores in Galaxy Clusters via Hierarchical Mergers","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Galaxy cluster; Adaptive mesh refinement; Substructure; Radiative cooling; Cluster (spacecraft); Galaxy formation and evolution; Cooling flow; Structure formation; Galaxy; Supercluster (genetic); Astronomy","score_opus":0.0066214529959667005,"score_gpt":0.21211007726090683,"score_spread":0.20548862426494013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966324939","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9869086,0.00006860155,0.0104688555,0.00006754719,0.000008420421,0.000023703109,0.0000285004,0.000102473976,0.0023231644],"genre_scores_gemma":[0.9950507,0.00005113676,0.004261771,0.00002688114,0.000004340382,0.000020450967,0.000035692883,0.000016907848,0.00053196825],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989057,0.00003117552,0.00000423674,0.000017917815,0.000025756368,0.000030254849],"domain_scores_gemma":[0.99970585,0.000094047915,0.00006528222,0.000029792334,0.000025636518,0.00007933856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034027992,0.0003004957,0.00026675675,0.00034148627,0.00058297,0.0008252945,0.00074658653,0.00048391684,0.0009947531],"category_scores_gemma":[0.0017951091,0.00032757557,0.0004567032,0.00020898528,0.0011349795,0.0006220734,0.0011839207,0.00038948187,0.00011565744],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012119652,0.00004882583,0.01914695,0.00002925207,0.000037516584,0.00027125576,0.0003460492,0.95875275,0.00522754,0.012830408,0.00023364405,0.0029547305],"study_design_scores_gemma":[0.000088477005,0.0000848195,0.0051409435,0.0000082629085,0.00001626774,0.000052594354,0.000094450785,0.9873037,0.00095271226,0.00569571,0.0005481863,0.000013880142],"about_ca_topic_score_codex":0.012709544,"about_ca_topic_score_gemma":0.009358962,"teacher_disagreement_score":0.012709544,"about_ca_system_score_codex":0.0008586278,"about_ca_system_score_gemma":0.00060873904,"threshold_uncertainty_score":0.025271177},"labels":[],"label_agreement":null},{"id":"W1966332592","doi":"10.1088/0004-637x/768/2/118","title":"A KINEMATIC APPROACH TO ASSESSING ENVIRONMENTAL EFFECTS: STAR-FORMING GALAXIES IN A<i>z</i>∼ 0.9 SpARCS CLUSTER USING<i>SPITZER</i>24 μm OBSERVATIONS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Population; Cluster (spacecraft); Stellar mass; Astronomy","score_opus":0.015623658389102953,"score_gpt":0.21752666248765903,"score_spread":0.20190300409855608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966332592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99398065,0.00010500949,0.0029593934,0.000015770369,0.0000021026297,0.000017518949,0.00083618454,0.000052781597,0.0020306315],"genre_scores_gemma":[0.9965224,0.000066592314,0.00228789,0.000011441992,0.0000072229695,0.000013330675,0.0008308285,0.000013826443,0.0002465438],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998222,0.00003302731,0.000013593123,0.000055187826,0.000042156804,0.000033892302],"domain_scores_gemma":[0.99932754,0.00010879526,0.00028848735,0.00007678421,0.00010470443,0.00009362527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034422745,0.00033789067,0.00017114852,0.0018867888,0.0003604701,0.00080545136,0.00041783167,0.00015029644,0.00057977607],"category_scores_gemma":[0.0009228768,0.0001866355,0.00022694512,0.0013145631,0.00035567945,0.0005142674,0.00059894245,0.00017050203,0.00020370918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004271842,0.000023448516,0.98725164,0.00001503801,0.000050306524,0.000050817893,0.00014546253,0.0011323941,0.006957605,0.00023657874,0.000067982925,0.004025977],"study_design_scores_gemma":[0.0000012462132,0.000029372217,0.9963092,0.0000030164013,0.000020899732,0.000046844725,0.00016157492,0.0013299058,0.0017401759,0.00007699628,0.0002763561,0.000004400359],"about_ca_topic_score_codex":0.008672927,"about_ca_topic_score_gemma":0.017819064,"teacher_disagreement_score":0.008672927,"about_ca_system_score_codex":0.00037364475,"about_ca_system_score_gemma":0.00026018568,"threshold_uncertainty_score":0.017244875},"labels":[],"label_agreement":null},{"id":"W1966373979","doi":"10.1086/375051","title":"Some Global Characteristics of the Galactic Globular Cluster System","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Metallicity; Galaxy; Astronomy; Dwarf galaxy; Luminosity; Galaxy cluster; Star cluster; Galaxy groups and clusters","score_opus":0.007185925345562493,"score_gpt":0.20779989543881366,"score_spread":0.20061397009325116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966373979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.969992,0.0007158672,0.0008289712,0.00018022009,0.000007729787,0.000019885207,0.0029449346,0.00006429936,0.025246112],"genre_scores_gemma":[0.9962948,0.00023682098,0.00027618743,0.000028097946,0.000013028806,0.0000072266935,0.0016213916,0.000019642408,0.0015027239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998783,0.000015886817,0.000009525679,0.00003829828,0.000026693373,0.00003124518],"domain_scores_gemma":[0.99924433,0.0001504592,0.00014827735,0.000065726934,0.00021826143,0.00017294426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021278528,0.00016341172,0.00021583415,0.0012894002,0.0003329034,0.0008457002,0.00022376471,0.00020968748,0.003628385],"category_scores_gemma":[0.0012170578,0.00010253317,0.00014159728,0.0017230725,0.00041299924,0.00060453336,0.0004867878,0.00018452699,0.00093393517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006537512,0.000012222623,0.97854656,0.00003209526,0.000044678276,0.000170178,0.00045934832,0.001319757,0.0030131936,0.001829148,0.0009250905,0.013582358],"study_design_scores_gemma":[0.0000013349443,0.00002239105,0.99579453,0.0000042608567,0.000010974215,0.00026804113,0.00018507162,0.00046152045,0.00016302355,0.00052685104,0.00255677,0.0000052403934],"about_ca_topic_score_codex":0.007993029,"about_ca_topic_score_gemma":0.010065564,"teacher_disagreement_score":0.007993029,"about_ca_system_score_codex":0.00050400244,"about_ca_system_score_gemma":0.00019568272,"threshold_uncertainty_score":0.015893042},"labels":[],"label_agreement":null},{"id":"W1966382893","doi":"10.1086/425853","title":"Probing Halos of Galaxies at Very Large Radii Using Background QSOs","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Quasar; QSOS; Redshift; Astronomy; Galaxy rotation curve; Halo; RADIUS","score_opus":0.014522009173974289,"score_gpt":0.22817279513158784,"score_spread":0.21365078595761355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966382893","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99940157,0.000046732082,0.00018290034,0.000005324102,4.5743403e-7,0.000002026879,0.00007770367,0.0000068904455,0.00027641267],"genre_scores_gemma":[0.99965286,0.00003607563,0.0001346675,0.000005701966,0.0000017296613,0.000001313248,0.00011880014,0.0000012731447,0.00004758098],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998785,0.000019509338,0.0000063977714,0.000036738278,0.000023151657,0.000035630957],"domain_scores_gemma":[0.99970216,0.00006299704,0.00006032997,0.00003233465,0.000030122224,0.0001120381],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024854837,0.0001765671,0.00019985068,0.000526898,0.00020810064,0.00058413914,0.00016692012,0.00012654997,0.0010504349],"category_scores_gemma":[0.00043263723,0.00013694348,0.00015558857,0.00045524363,0.0002714702,0.00027096286,0.000569859,0.0001306601,0.00012837796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047172,0.00007861716,0.86786485,0.00005164362,0.000100470825,0.00035571115,0.0008312386,0.0016415785,0.11903661,0.0006219354,0.00013043446,0.008815101],"study_design_scores_gemma":[0.0000107205715,0.000140134,0.9943152,0.000004204719,0.00003568167,0.00016699957,0.00029847448,0.0012737669,0.0032974107,0.00014313385,0.0003097957,0.0000044520602],"about_ca_topic_score_codex":0.003555542,"about_ca_topic_score_gemma":0.0046639624,"teacher_disagreement_score":0.003555542,"about_ca_system_score_codex":0.00024276554,"about_ca_system_score_gemma":0.000087227905,"threshold_uncertainty_score":0.007069707},"labels":[],"label_agreement":null},{"id":"W1966441755","doi":"10.1088/0004-637x/797/1/4","title":"A GENERAL HYBRID RADIATION TRANSPORT SCHEME FOR STAR FORMATION SIMULATIONS ON AN ADAPTIVE GRID","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Radiative transfer; Star formation; Thermal radiation; Radiation; Radiant energy; Diffusion; Stars; Convection; Radiation transport; Benchmark (surveying)","score_opus":0.01520801278322032,"score_gpt":0.2507070224335537,"score_spread":0.23549900965033338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966441755","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08321856,0.00027331733,0.8985159,0.00033601362,0.00017069509,0.00021659072,0.0007239644,0.0027989934,0.013746072],"genre_scores_gemma":[0.52241075,0.00021561456,0.46441212,0.00020298855,0.00006308414,0.0007734093,0.0009894694,0.00073668937,0.010195837],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998641,0.000035749978,0.000011559175,0.000020911088,0.00004679127,0.000020800067],"domain_scores_gemma":[0.99965096,0.00011359028,0.00003501726,0.000061788596,0.00009213615,0.00004651752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003852548,0.00052248524,0.0005124696,0.00030163093,0.00053946394,0.0006379888,0.0017692273,0.00096135534,0.004385396],"category_scores_gemma":[0.001114288,0.0003624748,0.0007191998,0.00046061203,0.0005693438,0.00059434486,0.001059749,0.0008938275,0.00075549097],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007100331,0.000044514978,0.0011518305,0.00005065486,0.000029114784,0.000105746,0.00007065752,0.9660928,0.005520483,0.012874996,0.0011601003,0.012827989],"study_design_scores_gemma":[0.000022480575,0.0000097185475,0.00007575128,0.0000029429748,0.000001923378,0.00000872561,0.0000047185254,0.99721634,0.00036631254,0.0012210798,0.0010654846,0.000004426599],"about_ca_topic_score_codex":0.009809585,"about_ca_topic_score_gemma":0.0065064263,"teacher_disagreement_score":0.009809585,"about_ca_system_score_codex":0.000839182,"about_ca_system_score_gemma":0.0011602632,"threshold_uncertainty_score":0.019504964},"labels":[],"label_agreement":null},{"id":"W1966456402","doi":"10.1088/0004-637x/795/1/86","title":"ON THE DIVERSITY OF MAGNETIC INTERACTIONS IN CLOSE-IN STAR-PLANET SYSTEMS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Planet; Astrophysics; Angular momentum; Stellar magnetic field; Stellar rotation; Planetary migration; Astronomy; Star (game theory); Exoplanet; Stars; Magnetic field; Solar wind; Classical mechanics; Coronal mass ejection","score_opus":0.009762753681394497,"score_gpt":0.20474647752308514,"score_spread":0.19498372384169063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966456402","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9891679,0.00064052024,0.0028473744,0.00027986206,0.00002163476,0.0000121604335,0.000078485326,0.000050784045,0.006901215],"genre_scores_gemma":[0.9990748,0.00018219062,0.00046584473,0.000017709272,0.000014582596,0.0000068113914,0.00005408407,0.000014089634,0.00016987846],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99978584,0.0000817687,0.000014776472,0.000043751355,0.000038026523,0.000035807712],"domain_scores_gemma":[0.9983543,0.00094643596,0.00024130801,0.00015325105,0.00010160807,0.00020302816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005145616,0.00029324056,0.0006902892,0.00083393406,0.0011012512,0.001500064,0.0006890357,0.00089144433,0.0013099374],"category_scores_gemma":[0.003859915,0.0002814984,0.0004165654,0.00050269236,0.001121444,0.001465115,0.0009842254,0.00045576427,0.00012539871],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024202782,0.0001961265,0.06360759,0.00018680694,0.00018215929,0.00082288234,0.00062003476,0.86540735,0.008456536,0.047813635,0.0014153776,0.0110495],"study_design_scores_gemma":[0.00007654323,0.000098217395,0.025152707,0.000040151994,0.00005391892,0.00029270776,0.00028509565,0.9378972,0.0010184646,0.033131253,0.001915193,0.0000386132],"about_ca_topic_score_codex":0.0014021771,"about_ca_topic_score_gemma":0.0014931003,"teacher_disagreement_score":0.001500064,"about_ca_system_score_codex":0.00050766364,"about_ca_system_score_gemma":0.00023204477,"threshold_uncertainty_score":0.0043821335},"labels":[],"label_agreement":null},{"id":"W1966516577","doi":"10.1086/522220","title":"The Black Hole Mass of NGC 4151: Comparison of Reverberation Mapping and Stellar Dynamical Measurements","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Black hole (networking); Stellar mass; Reverberation mapping; Rotational symmetry; Intermediate-mass black hole; Stellar black hole; Spectroscopy; Spin-flip; Galactic nuclei","score_opus":0.033366402351299305,"score_gpt":0.27066546281423515,"score_spread":0.23729906046293583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966516577","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99920386,0.000030321156,0.00032593406,0.00000703649,7.8052994e-7,0.0000014683784,0.000060135888,0.00002296365,0.00034746842],"genre_scores_gemma":[0.9996014,0.000020344261,0.00019235192,0.0000014359445,0.0000013924713,8.8069993e-7,0.00009866053,0.0000036827653,0.000079890044],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999417,0.000007728464,0.0000024957387,0.000023767912,0.000010941224,0.000013299916],"domain_scores_gemma":[0.99984086,0.000026458549,0.00006010121,0.000030006291,0.000014149753,0.000028385553],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001674864,0.00040234884,0.00014885253,0.0008602389,0.00022249101,0.00039424756,0.0003026625,0.00026880708,0.0008528803],"category_scores_gemma":[0.00039243308,0.0001443895,0.00022701565,0.000290759,0.00023512574,0.0003040626,0.000270595,0.00010362332,0.00018808074],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048447214,0.000083243925,0.8553589,0.00007847147,0.00014116368,0.00062724785,0.0011453767,0.01859391,0.088197194,0.0019054797,0.00032551694,0.03305911],"study_design_scores_gemma":[0.0000146518405,0.00006562317,0.96359897,0.0000062145614,0.00004879561,0.00020820404,0.000171011,0.028319238,0.0067661097,0.00043987014,0.00034507306,0.000016152322],"about_ca_topic_score_codex":0.0057074493,"about_ca_topic_score_gemma":0.005429324,"teacher_disagreement_score":0.0057074493,"about_ca_system_score_codex":0.0003727205,"about_ca_system_score_gemma":0.000080734564,"threshold_uncertainty_score":0.011348426},"labels":[],"label_agreement":null},{"id":"W1966560464","doi":"10.1088/0004-637x/778/1/78","title":"PLANETARY POPULATIONS IN THE MASS-PERIOD DIAGRAM: A STATISTICAL TREATMENT OF EXOPLANET FORMATION AND THE ROLE OF PLANET TRAPS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Exoplanet; Planet; Physics; Planetary migration; Astrophysics; Gas giant; Population; Accretion (finance); Planetary system; Planetary mass; Astrobiology; Astronomy","score_opus":0.012732027130687867,"score_gpt":0.23195784940954298,"score_spread":0.21922582227885512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966560464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7914606,0.00093696103,0.20252718,0.00046302142,0.000054786695,0.00004363296,0.00056549156,0.00027862116,0.003669734],"genre_scores_gemma":[0.9917999,0.0002550598,0.006839699,0.000041253854,0.000082116116,0.00005555168,0.00022008528,0.00006355028,0.0006426975],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99966323,0.00012426754,0.000015801077,0.00009898887,0.0000553362,0.00004239829],"domain_scores_gemma":[0.9942311,0.0035463702,0.0011563456,0.00059041235,0.0001978594,0.00027807467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016285317,0.00025590588,0.0003587491,0.0014768767,0.00038350563,0.0011540332,0.00060975866,0.0005730969,0.0013580163],"category_scores_gemma":[0.009080513,0.00015044083,0.00042843504,0.0009887301,0.0011350764,0.0016643339,0.0008249965,0.0007358207,0.00023922385],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024984838,0.00011760699,0.3440451,0.00013635517,0.000239278,0.00088215177,0.0018051725,0.23549892,0.01075256,0.3516571,0.0021572781,0.052458737],"study_design_scores_gemma":[0.000014915835,0.000113683556,0.08668049,0.000017223369,0.000038577247,0.00056305923,0.00021863545,0.82308894,0.0009231173,0.0840963,0.004199841,0.000045264896],"about_ca_topic_score_codex":0.0009273973,"about_ca_topic_score_gemma":0.00039233247,"teacher_disagreement_score":0.0016285317,"about_ca_system_score_codex":0.00042628363,"about_ca_system_score_gemma":0.00023240014,"threshold_uncertainty_score":0.008612633},"labels":[],"label_agreement":null},{"id":"W1966625802","doi":"10.1088/0004-637x/775/1/6","title":"THE CARINA PROJECT. VI. THE HELIUM-BURNING VARIABLE STARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Cepheid variable; RR Lyrae variable; Variable star; Diagram; Variable (mathematics); Instability strip; Distance modulus; Hertzsprung–Russell diagram","score_opus":0.009705440105965232,"score_gpt":0.21828728647099638,"score_spread":0.20858184636503113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966625802","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.06338841,0.03619875,0.028124398,0.006008182,0.0010301544,0.0008871442,0.58252245,0.0447759,0.23706454],"genre_scores_gemma":[0.18529144,0.0075370646,0.07595645,0.0016751947,0.0006689895,0.0016638266,0.6305032,0.012373451,0.084330365],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9989625,0.00026342983,0.000045279226,0.0002927128,0.0002682249,0.00016790784],"domain_scores_gemma":[0.99827206,0.000250061,0.0002682663,0.00046680003,0.0004264526,0.0003163462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021725108,0.0013599583,0.00066580577,0.003583824,0.0008579861,0.003455531,0.0014670087,0.00084056245,0.03329337],"category_scores_gemma":[0.0033149235,0.00045860372,0.000595291,0.0027331794,0.00036208594,0.0012632471,0.0028962616,0.0006775096,0.027903328],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001807862,0.0001563723,0.05016975,0.0020886788,0.00038745804,0.0004409887,0.0011176615,0.0016686228,0.0030988175,0.03027953,0.5470143,0.3617699],"study_design_scores_gemma":[0.000112826616,0.000040227766,0.021203954,0.00031733912,0.0000830609,0.00024293858,0.00016482234,0.0013101385,0.0010621255,0.0044170604,0.97101474,0.00003075294],"about_ca_topic_score_codex":0.027649917,"about_ca_topic_score_gemma":0.02181712,"teacher_disagreement_score":0.03329337,"about_ca_system_score_codex":0.0012019089,"about_ca_system_score_gemma":0.0016987523,"threshold_uncertainty_score":0.11137742},"labels":[],"label_agreement":null},{"id":"W1966684419","doi":"10.1088/0004-637x/712/2/1259","title":"THE ACS LCID PROJECT. II. FAINT VARIABLE STARS IN THE ISOLATED DWARF IRREGULAR GALAXY IC 1613","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; RR Lyrae variable; Physics; Astrophysics; Variable star; Astronomy; Photometry (optics); Light curve; Stars; Distance modulus; Galaxy; Large Magellanic Cloud; Overtone; Globular cluster; Spectral line","score_opus":0.008317877465467978,"score_gpt":0.22402961803666377,"score_spread":0.2157117405711958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966684419","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0009316251,0.0008411612,0.0035111816,0.00048337047,0.00033938987,0.00014374235,0.9243034,0.035744544,0.033701558],"genre_scores_gemma":[0.003711011,0.0007497864,0.009100639,0.0003052172,0.00016963224,0.00035381984,0.9691181,0.006296685,0.010195173],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9990952,0.00007990648,0.000059986156,0.00016234351,0.0004341034,0.00016839136],"domain_scores_gemma":[0.9986773,0.00013208562,0.00011224981,0.00038128375,0.0003657328,0.0003313502],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00151106,0.0020030634,0.0020863197,0.005134608,0.0013210821,0.00585662,0.0034013968,0.0013334316,0.20691584],"category_scores_gemma":[0.0029477053,0.0010516199,0.0012800772,0.007327404,0.00030670268,0.0024700088,0.003759628,0.0015941118,0.22348124],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009885795,0.000025387708,0.0010534887,0.00025680347,0.000033695662,0.000048419963,0.000034475263,0.000108282096,0.00048770814,0.0015574544,0.98087156,0.015423697],"study_design_scores_gemma":[0.00016249991,0.000011207222,0.004548166,0.0001165374,0.00004167917,0.000086786036,0.000038633756,0.00096317776,0.00085709174,0.0037723782,0.98937327,0.000028535685],"about_ca_topic_score_codex":0.018087374,"about_ca_topic_score_gemma":0.021854809,"teacher_disagreement_score":0.20691584,"about_ca_system_score_codex":0.0016502906,"about_ca_system_score_gemma":0.0020572913,"threshold_uncertainty_score":0.69220245},"labels":[],"label_agreement":null},{"id":"W1966697426","doi":"10.1088/0004-637x/774/1/58","title":"THE FAST AND FURIOUS DECAY OF THE PECULIAR TYPE Ic SUPERNOVA 2005ek","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Ejecta; Supernova; White dwarf; Light curve; Pair-instability supernova; Detonation; Spectral line","score_opus":0.0065162768784707585,"score_gpt":0.20786349948818542,"score_spread":0.20134722260971466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966697426","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955531,0.0002328368,0.00076876866,0.00002294504,0.000010959894,0.0000065915738,0.00050344213,0.000041406653,0.00285995],"genre_scores_gemma":[0.9968516,0.00012872637,0.0010738372,0.000054422086,0.000014087833,0.000003975619,0.0011973626,0.000010984828,0.0006650196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999182,0.0000035541975,0.000005039749,0.000031067048,0.000021228621,0.000020956883],"domain_scores_gemma":[0.9998605,0.000009653191,0.000049806353,0.000021755444,0.000022124674,0.00003602028],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018772886,0.00019593381,0.00017813181,0.00048804737,0.00030169764,0.0004886567,0.00024519104,0.00019318167,0.0005157052],"category_scores_gemma":[0.00028692602,0.00009867621,0.00017192577,0.0002637649,0.0001556638,0.00023748557,0.00036970802,0.00023861382,0.00016475443],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034540019,0.000108057655,0.8162076,0.00011465604,0.00017713824,0.0018123133,0.0003594354,0.0007903454,0.13978164,0.0017419251,0.0017683982,0.036793046],"study_design_scores_gemma":[0.0000030186038,0.00006171112,0.9891306,0.0000110878345,0.000023462515,0.0012889067,0.000082247556,0.0004128824,0.0047140014,0.00013478498,0.004130277,0.0000069484954],"about_ca_topic_score_codex":0.0029569834,"about_ca_topic_score_gemma":0.00570363,"teacher_disagreement_score":0.0029569834,"about_ca_system_score_codex":0.00024399167,"about_ca_system_score_gemma":0.00013373679,"threshold_uncertainty_score":0.0058795214},"labels":[],"label_agreement":null},{"id":"W1966785550","doi":"10.1086/513180","title":"A New Algorithm for Point‐Spread Function Subtraction in High‐Contrast Imaging: A Demonstration with Angular Differential Imaging","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":461,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Point spread function; Residual; Subtraction; Speckle pattern; Differential (mechanical device); Noise (video); Sensitivity (control systems); Function (biology)","score_opus":0.005221664586165699,"score_gpt":0.21210900702011784,"score_spread":0.20688734243395215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966785550","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0027454023,0.000042156607,0.996024,0.000034632725,0.000021777734,0.000023201652,0.000016170923,0.00062260934,0.00047004636],"genre_scores_gemma":[0.016170127,0.000052708114,0.98272943,0.000030685525,0.00001826714,0.000039889474,0.00007985616,0.00009638061,0.00078259344],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994074,0.00006215559,0.000030749474,0.00012011681,0.00033420077,0.00004543451],"domain_scores_gemma":[0.99919933,0.00018525159,0.000065093576,0.00018319552,0.00032301576,0.00004421454],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008577895,0.0007106521,0.00060177024,0.00079873187,0.00048814507,0.0012205389,0.0016845142,0.0008878342,0.0017842351],"category_scores_gemma":[0.0015846412,0.0005474339,0.0006984916,0.00076520257,0.0005620942,0.0011876,0.0011866044,0.0012748531,0.0019410896],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022460982,0.0001258986,0.00136208,0.000118804484,0.00010649179,0.00015622677,0.00013968769,0.03559848,0.16730827,0.013466016,0.0033386163,0.7780549],"study_design_scores_gemma":[0.0000780002,0.00015673984,0.0026853874,0.000016528074,0.000057093603,0.0009811359,0.000043731787,0.8599816,0.1076436,0.0073735346,0.020884873,0.00009775321],"about_ca_topic_score_codex":0.0017333729,"about_ca_topic_score_gemma":0.0027967468,"teacher_disagreement_score":0.0017842351,"about_ca_system_score_codex":0.00045028015,"about_ca_system_score_gemma":0.0007542795,"threshold_uncertainty_score":0.0059688687},"labels":[],"label_agreement":null},{"id":"W1966902691","doi":"10.1086/523661","title":"An Explanation for the Observed Weak Size Evolution of Disk Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":178,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Los Alamos National Laboratory; U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; University of Pittsburgh; Johns Hopkins University; University of Chicago; U.S. Department of Energy; Princeton University; Space Telescope Science Institute; New Mexico State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Dark matter; Stellar mass; Redshift; Astronomy; Galaxy formation and evolution; Halo; Virial theorem; Dark matter halo; Star formation","score_opus":0.016959163480555383,"score_gpt":0.2225283259933051,"score_spread":0.20556916251274973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1966902691","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9665995,0.0014786487,0.01932571,0.0019259099,0.000045579305,0.000026786387,0.0010616117,0.00044570552,0.009090468],"genre_scores_gemma":[0.9977677,0.0000952199,0.0009633791,0.00009069359,0.000010336825,0.0000047410854,0.00016626388,0.000011899712,0.00088983617],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998671,0.000010305161,0.0000060321254,0.0000701744,0.00002011065,0.000026207506],"domain_scores_gemma":[0.99939597,0.00014636607,0.00017269772,0.000098421304,0.00009988374,0.00008662306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023272254,0.00029830835,0.0001996248,0.00050692743,0.00038585128,0.00044019968,0.00076884555,0.0005961751,0.0040780045],"category_scores_gemma":[0.0013593995,0.00022885096,0.00028608114,0.0004630399,0.00064746494,0.00074519333,0.0005268307,0.00036944184,0.0007544923],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001894846,0.00009969086,0.8932671,0.00019891972,0.000087474065,0.0005438025,0.00049633865,0.010974271,0.03964212,0.020286966,0.002329955,0.03188398],"study_design_scores_gemma":[0.000037246467,0.00010726548,0.9573567,0.0000136334775,0.000025447236,0.00096347765,0.00011864558,0.018172868,0.0072468966,0.012705613,0.003233665,0.000018466282],"about_ca_topic_score_codex":0.006351401,"about_ca_topic_score_gemma":0.006279833,"teacher_disagreement_score":0.006351401,"about_ca_system_score_codex":0.000641783,"about_ca_system_score_gemma":0.0002282863,"threshold_uncertainty_score":0.0136422515},"labels":[],"label_agreement":null},{"id":"W1967137800","doi":"10.1086/503321","title":"TeV Gamma‐Ray Observations of the Perseus and Abell 2029 Galaxy Clusters","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Cosmic ray; Galaxy cluster; Galaxy; Gamma ray; Surface brightness; Astronomy; Dark matter; Spectral index; Annihilation; Flux (metallurgy); Cluster (spacecraft); Astroparticle physics; Spectral line; Nuclear physics","score_opus":0.00892450750141356,"score_gpt":0.19845993570929438,"score_spread":0.18953542820788083,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967137800","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99862695,0.000047315152,0.00008456762,0.000011270779,0.000001597328,0.0000025458617,0.00017611578,0.000015345899,0.0010344194],"genre_scores_gemma":[0.99884796,0.000039030667,0.00025733994,0.000011157515,0.0000040877167,0.000003575773,0.00056427065,0.0000034272332,0.00026918424],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991345,0.00001153082,0.000004830561,0.000024161489,0.000023959956,0.00002205691],"domain_scores_gemma":[0.99971515,0.000036159,0.00009712791,0.00003665539,0.000037037815,0.00007781408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016705529,0.00022906205,0.00015542888,0.0009422043,0.00041810898,0.0003203154,0.00014468486,0.00015742396,0.000639625],"category_scores_gemma":[0.0004204752,0.00011923988,0.00010025981,0.00056376134,0.00021054753,0.0001262909,0.00040297088,0.0001341405,0.00014972572],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070678804,0.00008149831,0.9147631,0.000038520502,0.000092935086,0.0006874626,0.0006357815,0.002612535,0.062102247,0.0010324254,0.0016328149,0.015613925],"study_design_scores_gemma":[0.000009179269,0.000024926034,0.99621373,0.0000036702704,0.0000075099633,0.00011379763,0.0000722325,0.00047622918,0.002287285,0.000104107676,0.0006832281,0.000004084467],"about_ca_topic_score_codex":0.010714945,"about_ca_topic_score_gemma":0.019386297,"teacher_disagreement_score":0.010714945,"about_ca_system_score_codex":0.0005775421,"about_ca_system_score_gemma":0.00012528757,"threshold_uncertainty_score":0.021305144},"labels":[],"label_agreement":null},{"id":"W1967170472","doi":"10.1088/0004-637x/777/1/10","title":"SHORT TIMESCALE VARIATIONS IN THE ATMOSPHERE OF ANTARES A","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Variation (astronomy); Astrophysics; Atmosphere (unit); Convection; Line (geometry); Solar atmosphere; Radial velocity; Astronomy; Atmospheric sciences; Stars; Meteorology","score_opus":0.008581371395630585,"score_gpt":0.2175059761728259,"score_spread":0.20892460477719532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967170472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99836284,0.00020355955,0.00018175198,0.000048978985,0.000009108136,0.000002560785,0.00030694218,0.000033495315,0.0008506708],"genre_scores_gemma":[0.9986865,0.00009120543,0.0002934524,0.000022526518,0.000019324667,0.0000035098715,0.00071883574,0.000014215672,0.00015054179],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999051,0.000009201375,0.0000050971735,0.00003932093,0.000025138123,0.000016111888],"domain_scores_gemma":[0.99974483,0.00004625954,0.00008532679,0.000022750328,0.000043906974,0.000056935707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018883328,0.00013954597,0.00019158871,0.00063433795,0.00043544956,0.00063323823,0.0002095146,0.0004374326,0.00050300197],"category_scores_gemma":[0.0005611085,0.00013006543,0.00021062765,0.00048759513,0.0002095959,0.0003774101,0.00043637934,0.00027436545,0.00018548997],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029133537,0.00023664435,0.8414817,0.0001124016,0.00039531873,0.000607511,0.0011072332,0.005781981,0.117370375,0.0009850755,0.0019255357,0.02970492],"study_design_scores_gemma":[0.0000067318815,0.000039732444,0.9940633,0.0000037301174,0.000026403679,0.00010235954,0.00010152133,0.0031060579,0.00066630705,0.00017246648,0.0017010926,0.000010348709],"about_ca_topic_score_codex":0.004759632,"about_ca_topic_score_gemma":0.0065778675,"teacher_disagreement_score":0.004759632,"about_ca_system_score_codex":0.00029521482,"about_ca_system_score_gemma":0.00012639043,"threshold_uncertainty_score":0.009463847},"labels":[],"label_agreement":null},{"id":"W1967176793","doi":"10.1086/513712","title":"Lost and Found: A New Position and Infrared Counterpart for the X‐Ray Binary Scutum X‐1","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; X-ray binary; Neutron star; Extinction (optical mineralogy); Supergiant; Binary number; Infrared; X-ray; Pulsar; Astronomy; Optics; Stars","score_opus":0.012201672104648623,"score_gpt":0.24644906186273444,"score_spread":0.23424738975808582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967176793","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99739444,0.00021934943,0.00015217891,0.00008602562,0.000024277186,0.000007753752,0.000116358366,0.000021402424,0.0019780921],"genre_scores_gemma":[0.9978604,0.000063969106,0.0004067365,0.000059517708,0.000029638693,0.0000053616736,0.00052017154,0.000008221426,0.0010461361],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997683,0.000010384127,0.000014397902,0.00008157986,0.00006460444,0.000060702994],"domain_scores_gemma":[0.9994562,0.0000409706,0.00019370267,0.00007895151,0.000073215546,0.00015680343],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002138598,0.00021325791,0.00035841836,0.0015979861,0.0017088922,0.0012972233,0.00038490145,0.0005468185,0.002151027],"category_scores_gemma":[0.00084407115,0.00014990858,0.00012209715,0.0013325189,0.0005643167,0.0004639571,0.0011005873,0.0005796457,0.00048564046],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005730926,0.00030910305,0.8750875,0.00016944365,0.00005789493,0.00862894,0.004802653,0.00017431378,0.04293683,0.00278397,0.0022766166,0.062199686],"study_design_scores_gemma":[0.00002632714,0.0002601378,0.97973585,0.00003850618,0.000025755586,0.006437662,0.0006900721,0.0005052979,0.0019365125,0.00047570173,0.0098564355,0.000011752741],"about_ca_topic_score_codex":0.0046156365,"about_ca_topic_score_gemma":0.0061299815,"teacher_disagreement_score":0.0046156365,"about_ca_system_score_codex":0.00056759967,"about_ca_system_score_gemma":0.0003774907,"threshold_uncertainty_score":0.009177566},"labels":[],"label_agreement":null},{"id":"W1967182202","doi":"10.1088/0004-637x/738/1/101","title":"THE GLOBAL EVOLUTION OF GIANT MOLECULAR CLOUDS. II. THE ROLE OF ACCRETION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Molecular cloud; Physics; Astrophysics; Star formation; Accretion (finance); Virial theorem; Milky Way; Protostar; Galaxy; Astronomy; Star cluster; Stars","score_opus":0.00641235394559891,"score_gpt":0.21220286615438164,"score_spread":0.20579051220878272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967182202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9546284,0.0074229343,0.023366133,0.0009455155,0.000043485878,0.000026938853,0.00049413956,0.00017830994,0.012894132],"genre_scores_gemma":[0.9945433,0.0019503395,0.0024983613,0.00006014115,0.000022570359,0.000011482322,0.00015430001,0.000026107025,0.00073342765],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999969,0.0000052094924,0.0000012020091,0.000008296719,0.000005386656,0.000010879073],"domain_scores_gemma":[0.99989116,0.000019673293,0.00005137861,0.000012297561,0.000008825905,0.000016695009],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013429651,0.00036112362,0.00017412593,0.0003440834,0.00025341572,0.0008112686,0.00028874242,0.00044796575,0.00060879294],"category_scores_gemma":[0.000477544,0.00018657144,0.0003265444,0.00040402715,0.00044744933,0.0011135812,0.00053684943,0.0002432231,0.00018539908],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014795236,0.00003828897,0.31055132,0.00042332118,0.00022260993,0.0008581707,0.0009009479,0.43401912,0.0300325,0.15537342,0.0026077775,0.064824566],"study_design_scores_gemma":[0.000057449077,0.00018002892,0.3373475,0.00018477721,0.00022853135,0.0012133135,0.0006483919,0.49241075,0.006685079,0.13308564,0.027891977,0.00006656961],"about_ca_topic_score_codex":0.0030874105,"about_ca_topic_score_gemma":0.0028638327,"teacher_disagreement_score":0.0030874105,"about_ca_system_score_codex":0.0009062427,"about_ca_system_score_gemma":0.00024434042,"threshold_uncertainty_score":0.0065752864},"labels":[],"label_agreement":null},{"id":"W1967205217","doi":"10.1086/308413","title":"Young Globular Clusters and Dwarf Spheroidals","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Astronomy; Galactic halo; Halo; Galaxy; Dwarf spheroidal galaxy; Dwarf galaxy; Elliptical galaxy; Galaxy group","score_opus":0.0069622223636680814,"score_gpt":0.21046525204421726,"score_spread":0.20350302968054917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967205217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9641717,0.014604772,0.0016450243,0.0006544965,0.0000782776,0.000012708852,0.00017234964,0.000042018542,0.018618634],"genre_scores_gemma":[0.9884122,0.00357405,0.00039975217,0.00010745648,0.00006880081,0.0000030916683,0.00021651089,0.000004399753,0.0072138263],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.0000076804445,0.0000030732633,0.00002395473,0.000015847792,0.000020474348],"domain_scores_gemma":[0.9992874,0.000120589364,0.00022606927,0.000045899462,0.000085705455,0.00023437307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023921087,0.00009555987,0.0001718186,0.00035800858,0.00040117017,0.000502449,0.00016203808,0.00021645344,0.0018343847],"category_scores_gemma":[0.00077450334,0.0000730079,0.000050395927,0.00052471564,0.0005604401,0.00049079774,0.000422314,0.0001498587,0.0002901329],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039039511,0.00005093827,0.7189933,0.00035827677,0.000047711277,0.002567973,0.0033269173,0.0017299731,0.014687658,0.12391442,0.009099177,0.12483314],"study_design_scores_gemma":[0.000026862144,0.00009454321,0.89000154,0.000094695344,0.000024217756,0.0023346741,0.0011611349,0.00094820914,0.0015561095,0.04341572,0.06032097,0.000021389385],"about_ca_topic_score_codex":0.00624052,"about_ca_topic_score_gemma":0.008355857,"teacher_disagreement_score":0.00624052,"about_ca_system_score_codex":0.0005167673,"about_ca_system_score_gemma":0.00037334155,"threshold_uncertainty_score":0.012408376},"labels":[],"label_agreement":null},{"id":"W1967242449","doi":"10.1086/512064","title":"Infrared Excess Sources in the Canadian Galactic Plane Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Galactic plane; Infrared; Cosmic dust; Interstellar medium; Photodissociation; Interstellar cloud; Astrochemistry; Population; Hydrogen molecule; Astronomy; Hydrogen; Galaxy; Stars; Photochemistry","score_opus":0.017121008128738457,"score_gpt":0.25035343571710755,"score_spread":0.2332324275883691,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967242449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9297673,0.0015729433,0.0005186754,0.0004144604,0.00002024972,0.00007209928,0.052781843,0.00007479515,0.014777642],"genre_scores_gemma":[0.9697623,0.0010437923,0.0012063723,0.00013612145,0.000011341664,0.000037372898,0.024679754,0.000019395797,0.0031035673],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992099,0.000028604802,0.000025360341,0.0001393524,0.00038054396,0.0002162073],"domain_scores_gemma":[0.99815303,0.00005486986,0.00025109455,0.00008953922,0.0012022954,0.00024917212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042058423,0.0003241233,0.00030070235,0.004293348,0.002185803,0.0010427039,0.0007055071,0.00022035051,0.0028767474],"category_scores_gemma":[0.001689992,0.00023405123,0.00021553965,0.009160339,0.00029089485,0.00027247344,0.00096409285,0.00027039743,0.00040738625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000104144194,0.000018049095,0.96844226,0.000068724315,0.00008129964,0.00015374216,0.0007454596,0.00034695765,0.0016061622,0.00070072006,0.0102626635,0.017469853],"study_design_scores_gemma":[0.0000026621967,0.0000031118236,0.99423474,0.000013167366,0.00001777197,0.000064770655,0.000237309,0.00012089631,0.00014098399,0.000028232884,0.0051276106,0.000008782992],"about_ca_topic_score_codex":0.9909025,"about_ca_topic_score_gemma":0.9960886,"teacher_disagreement_score":0.9909025,"about_ca_system_score_codex":0.010493774,"about_ca_system_score_gemma":0.009549747,"threshold_uncertainty_score":0.07613796},"labels":[],"label_agreement":null},{"id":"W1967288315","doi":"10.1088/0004-637x/755/1/70","title":"A MEASUREMENT OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH TWO YEARS OF SOUTH POLE TELESCOPE OBSERVATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":259,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; University of Chicago; McGill University; U.S. Department of Energy; Gordon and Betty Moore Foundation; National Science Foundation; Yale University; Office of Science; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Cosmic microwave background; Cosmic infrared background; South Pole Telescope; Spectral density; Anisotropy; Thermal; Amplitude; Cosmic background radiation","score_opus":0.02221941622358224,"score_gpt":0.2197798713169819,"score_spread":0.19756045509339967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967288315","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99760985,0.000032228963,0.00082928024,0.000033808083,0.000004402835,0.0000051595116,0.00041461087,0.000021433152,0.0010490984],"genre_scores_gemma":[0.99878746,0.000013798447,0.0005177204,0.0000075892726,0.000007254799,0.0000047083695,0.0005531966,0.000004825756,0.0001034413],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998012,0.000033603545,0.0000082670695,0.000058451733,0.00006446655,0.000034047673],"domain_scores_gemma":[0.99918073,0.00012122829,0.00025563632,0.00014814042,0.00013021893,0.0001640447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045125344,0.00027318875,0.00017727984,0.0006095533,0.00029400788,0.0004178982,0.00022212516,0.00026314624,0.0008518829],"category_scores_gemma":[0.0013068233,0.00023894438,0.0002666217,0.0005284962,0.00018884336,0.000292223,0.00036675998,0.00031377256,0.00022840212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025867723,0.000048204212,0.9547103,0.000027445742,0.00012324224,0.00011876846,0.00028729133,0.0012093098,0.034380425,0.00033032626,0.00061698176,0.007889012],"study_design_scores_gemma":[0.00000482797,0.000020631353,0.99672914,0.0000016620348,0.00001611913,0.000029014544,0.000013235862,0.0011877501,0.0014623104,0.000029943189,0.0005023781,0.0000030506187],"about_ca_topic_score_codex":0.005895801,"about_ca_topic_score_gemma":0.011967609,"teacher_disagreement_score":0.005895801,"about_ca_system_score_codex":0.00046942063,"about_ca_system_score_gemma":0.00014600047,"threshold_uncertainty_score":0.011722982},"labels":[],"label_agreement":null},{"id":"W1967382316","doi":"10.1086/522030","title":"Predicted and Observed Evolution in the Mean Properties of Type Ia Supernovae with Redshift","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Supernova; Astrophysics; Redshift; Galaxy; Luminosity; Dark energy; Population; COSMIC cancer database; Star formation; Type (biology); Cosmology; Astronomy","score_opus":0.019420811831784242,"score_gpt":0.2216077130183877,"score_spread":0.20218690118660346,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967382316","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913749,0.00025460232,0.0042784708,0.000039008504,0.0000060778307,0.0000113099995,0.0020341668,0.00018863866,0.001812907],"genre_scores_gemma":[0.99534297,0.00014118827,0.0013646969,0.000014563194,0.0000066097264,0.0000121813555,0.002537254,0.000031139338,0.000549388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999759,0.000040381467,0.000022573044,0.00010559658,0.000039133574,0.000033362357],"domain_scores_gemma":[0.99579287,0.0015677892,0.0011625453,0.0005338659,0.0007168702,0.00022609204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011132965,0.00026595197,0.00020524902,0.000876935,0.0001855903,0.00085978204,0.00044308623,0.00036434166,0.0023562843],"category_scores_gemma":[0.0055343644,0.00022224762,0.00044402407,0.0006883692,0.00026081133,0.0006542659,0.00020770617,0.0002878727,0.0010173159],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006160208,0.000016141375,0.9865846,0.00001808112,0.000055980472,0.000028232898,0.00003518077,0.0039718933,0.0029655963,0.00051242544,0.0001608614,0.0055894423],"study_design_scores_gemma":[0.0000037843863,0.00005420147,0.9894683,0.000005729789,0.00002126513,0.00015517353,0.000024064375,0.007270088,0.001768344,0.0005953761,0.0006248587,0.0000089601335],"about_ca_topic_score_codex":0.0018391273,"about_ca_topic_score_gemma":0.002339872,"teacher_disagreement_score":0.0023562843,"about_ca_system_score_codex":0.0005567444,"about_ca_system_score_gemma":0.00013965539,"threshold_uncertainty_score":0.007882595},"labels":[],"label_agreement":null},{"id":"W1967390719","doi":"10.1086/508504","title":"The Chemical Evolution of Helium in Globular Clusters: Implications for the Self‐Pollution Scenario","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Helium; Stellar evolution; Asymptotic giant branch; Stars; Horizontal branch; Stellar collision; Giant star; Hertzsprung–Russell diagram","score_opus":0.007228897595232862,"score_gpt":0.22161080050338583,"score_spread":0.21438190290815295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967390719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983631,0.000058262543,0.00046759163,0.00017820399,0.000002373907,0.0000018432163,0.000011598405,0.000005024862,0.00091205636],"genre_scores_gemma":[0.9995408,0.000054221855,0.00012533365,0.000018017596,0.0000033768001,8.0002445e-7,0.000011114769,0.0000017511193,0.00024468123],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996734,0.0000083142095,0.0000015150662,0.0000067332257,0.00000662787,0.000009386331],"domain_scores_gemma":[0.9995908,0.00013375949,0.000103846454,0.000038619804,0.00005283209,0.00008021801],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032860902,0.00015542723,0.00014225378,0.00044849407,0.00066743337,0.0007101592,0.00055202097,0.00066780724,0.0009170846],"category_scores_gemma":[0.0009131717,0.00013047647,0.00021185486,0.00037888542,0.0008554144,0.00072815106,0.0006827901,0.00022314706,0.00011066171],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051978836,0.00014790568,0.73593867,0.00007212136,0.00011263762,0.001755294,0.0011980543,0.13677338,0.026935656,0.08254644,0.0010394072,0.012960637],"study_design_scores_gemma":[0.00012184287,0.0002975311,0.51090693,0.000021501355,0.00008384718,0.0009225091,0.0016357377,0.36297953,0.0072266385,0.11383735,0.0019026742,0.00006387657],"about_ca_topic_score_codex":0.006242868,"about_ca_topic_score_gemma":0.0047540828,"teacher_disagreement_score":0.006242868,"about_ca_system_score_codex":0.0009868179,"about_ca_system_score_gemma":0.00029800247,"threshold_uncertainty_score":0.0124130845},"labels":[],"label_agreement":null},{"id":"W1967461765","doi":"10.1086/589830","title":"Molecular Gas in the <i>z</i> = 1.2 Ultraluminous Merger GOODS J123634.53+621241.3","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Galaxy; Luminous infrared galaxy; Star formation; Spiral galaxy; Redshift; Luminosity; Galaxy merger; Line (geometry)","score_opus":0.00785169003695544,"score_gpt":0.20610972025839344,"score_spread":0.198258030221438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967461765","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99927205,0.00010772439,0.000034745663,0.0000146097955,0.000001929642,0.0000017332832,0.0000588038,0.000011676817,0.00049677305],"genre_scores_gemma":[0.99940765,0.000048191083,0.00011014849,0.00001888904,0.0000051422394,0.0000031823984,0.00024028421,0.0000038708904,0.00016273194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998722,0.000008964021,0.0000039835686,0.00003274144,0.000027516524,0.000054575023],"domain_scores_gemma":[0.99987304,0.000008454658,0.00006888166,0.000007884787,0.000009926325,0.000031854186],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012638705,0.00019269912,0.00025893052,0.0006371238,0.00047211625,0.00068575825,0.00045561197,0.0003531082,0.00063631916],"category_scores_gemma":[0.00020101144,0.00018555472,0.00012879337,0.00049345446,0.0003193829,0.00022013507,0.0006305703,0.00025297154,0.0002951501],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004933698,0.00016070619,0.8247996,0.000066901775,0.00009780687,0.0012607703,0.00063237245,0.00036961597,0.15767214,0.000546407,0.001166217,0.012734033],"study_design_scores_gemma":[0.000013906467,0.000050328414,0.9938606,0.000004657666,0.00003363387,0.00046981935,0.00014798425,0.00044926838,0.0036531794,0.0000781016,0.0012311568,0.000007334192],"about_ca_topic_score_codex":0.0062329248,"about_ca_topic_score_gemma":0.0071929605,"teacher_disagreement_score":0.0062329248,"about_ca_system_score_codex":0.0005088792,"about_ca_system_score_gemma":0.00009925357,"threshold_uncertainty_score":0.012393296},"labels":[],"label_agreement":null},{"id":"W1967467143","doi":"10.1086/317278","title":"Precursors of Gamma-Ray Bursts: A Clue to the Burster’s Nature","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Photosphere; Thermal; Gamma-ray burst; Photon; Emission spectrum; Instability","score_opus":0.006209200166319371,"score_gpt":0.230890935452779,"score_spread":0.22468173528645963,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967467143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94035953,0.023455458,0.006798208,0.006289477,0.0006215381,0.000049001603,0.0005598377,0.0002067892,0.021660106],"genre_scores_gemma":[0.9854571,0.006320719,0.0028880406,0.0010657078,0.00055525894,0.000023273768,0.00029877457,0.000068696456,0.0033224982],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996823,0.00007483817,0.00003397191,0.00009523653,0.00006635425,0.00004725899],"domain_scores_gemma":[0.99534446,0.0018991198,0.0009783792,0.0006401264,0.0005306012,0.00060726237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009704433,0.0002422273,0.00032720756,0.0011867412,0.00058736664,0.0026584514,0.0005778331,0.0015200169,0.0023844333],"category_scores_gemma":[0.0052071516,0.00024829092,0.00015432364,0.00054024585,0.0011178874,0.0025466233,0.0011357572,0.0013287214,0.000668899],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023071459,0.0002022829,0.55240935,0.00072741916,0.00011107913,0.0076256543,0.008089765,0.00052643166,0.106530875,0.09196388,0.0054318514,0.22407424],"study_design_scores_gemma":[0.00011529736,0.00080733036,0.7089865,0.00083945313,0.00025603976,0.05232468,0.010072895,0.0024188347,0.032986294,0.08524444,0.105807886,0.00014026742],"about_ca_topic_score_codex":0.00051235943,"about_ca_topic_score_gemma":0.0003503626,"teacher_disagreement_score":0.0026584514,"about_ca_system_score_codex":0.0002449338,"about_ca_system_score_gemma":0.00025696063,"threshold_uncertainty_score":0.007976711},"labels":[],"label_agreement":null},{"id":"W1967633346","doi":"10.1086/368076","title":"Around‐the‐Clock Observations of the Q0957+561A,B Gravitationally Lensed Quasar. II. Results for the Second Observing Season","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Quasar; Brightness; Physics; Astrophysics; Ephemeris; Astronomy; Surface brightness; Epoch (astronomy); Galaxy","score_opus":0.02352432789033125,"score_gpt":0.23267430357701196,"score_spread":0.2091499756866807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967633346","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937895,0.000103366125,0.00036220683,0.000049999657,0.000010936255,0.000053502325,0.0040026708,0.000033386328,0.0015944238],"genre_scores_gemma":[0.9694216,0.0001591015,0.002472673,0.000109579574,0.00004451603,0.00012351926,0.025035392,0.000042755404,0.0025908276],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999549,0.000038282265,0.000038945098,0.00009135604,0.000100607875,0.00018187666],"domain_scores_gemma":[0.99862444,0.00020894497,0.00034882047,0.0002094605,0.0002569756,0.00035134144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076237123,0.00044902533,0.0005047079,0.0012705269,0.00059105817,0.0005978967,0.00031214496,0.0004177094,0.0013239703],"category_scores_gemma":[0.0009030793,0.00022484257,0.00052931724,0.0005648416,0.00018427396,0.00029458306,0.0006604327,0.00043406553,0.0008538581],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013185634,0.0006296461,0.946222,0.00007397024,0.00012746608,0.00047221503,0.000613668,0.0007353727,0.031762987,0.00020695373,0.0021658698,0.015671384],"study_design_scores_gemma":[0.000030223151,0.00015057556,0.9966792,0.000003545385,0.000025600324,0.00012667419,0.00008703715,0.00022620718,0.0014752187,0.000017314533,0.0011711996,0.000007301765],"about_ca_topic_score_codex":0.022527589,"about_ca_topic_score_gemma":0.038525283,"teacher_disagreement_score":0.022527589,"about_ca_system_score_codex":0.00038034894,"about_ca_system_score_gemma":0.00033334075,"threshold_uncertainty_score":0.04479289},"labels":[],"label_agreement":null},{"id":"W1967664515","doi":"10.1086/498820","title":"A High‐Resolution Map of<sup>12</sup>CO<i>J</i>= 6–5 Emission in the Starburst Galaxy M82","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Excitation; Galaxy; James Clerk Maxwell Telescope; Outflow; Angular resolution (graph drawing); Telescope; Mean kinetic temperature; Resolution (logic); Excitation temperature","score_opus":0.005981241164392668,"score_gpt":0.20500060581541188,"score_spread":0.19901936465101921,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967664515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99131936,0.00018927624,0.0011285485,0.00011230622,0.0000043895375,0.0000055140945,0.0013201255,0.00021362666,0.005706871],"genre_scores_gemma":[0.99360293,0.00013839663,0.0027944495,0.000038935097,0.00002684226,0.0000095190335,0.0015764761,0.000047112324,0.0017653321],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999727,0.0000017698627,9.321168e-7,0.000007148004,0.000008023774,0.000009419416],"domain_scores_gemma":[0.99988437,0.000011396031,0.000027323948,0.000014099866,0.000032413664,0.000030444648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000042602467,0.00009790689,0.000102587255,0.0006388531,0.00020853922,0.00036346013,0.00014755075,0.0002132152,0.0032336123],"category_scores_gemma":[0.00013444539,0.00013753536,0.00012355023,0.00044277275,0.000080443766,0.0001191444,0.00020818022,0.00016858232,0.0007053572],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054402335,0.00009985925,0.21556109,0.00022960496,0.00010887421,0.002032418,0.0013305884,0.0059178337,0.6982552,0.0009460621,0.0077110147,0.06726344],"study_design_scores_gemma":[0.00000877713,0.000034807475,0.98695564,0.00001664668,0.000023193586,0.00048260362,0.00015509999,0.0015881466,0.005046188,0.00010579926,0.0055748094,0.000008276745],"about_ca_topic_score_codex":0.004317167,"about_ca_topic_score_gemma":0.009097959,"teacher_disagreement_score":0.004317167,"about_ca_system_score_codex":0.0001326118,"about_ca_system_score_gemma":0.00010924326,"threshold_uncertainty_score":0.010817528},"labels":[],"label_agreement":null},{"id":"W1967713828","doi":"10.1088/0004-637x/777/2/106","title":"STELLAR COLLISIONS AND BLUE STRAGGLER STARS IN DENSE GLOBULAR CLUSTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Black Holes and Theoretical Physics","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada; Space Telescope Science Institute; University of Florida; Aspen Center for Physics; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Northwestern University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Globular cluster; Blue straggler; Binary number; Stars; Star cluster; Cluster (spacecraft); Stellar collision; Binary star; Population","score_opus":0.005765409344860265,"score_gpt":0.2126014013898798,"score_spread":0.2068359920450195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967713828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977609,0.00005867636,0.001520589,0.000030052868,0.000001990381,0.000005963998,0.000040788294,0.00002838432,0.00055264373],"genre_scores_gemma":[0.99917275,0.000054657692,0.0003122821,0.0000067270607,0.0000028757224,0.0000046963623,0.000057299785,0.000009937107,0.00037877125],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998622,0.00004049045,0.000006831858,0.000028784822,0.000026343092,0.000035389898],"domain_scores_gemma":[0.99912566,0.0003927091,0.00024084469,0.000045994646,0.00004047201,0.00015431165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050041097,0.00048099336,0.00038077845,0.00075127237,0.0007417059,0.00094001915,0.00077252346,0.0007677711,0.00085564016],"category_scores_gemma":[0.00184097,0.00043601924,0.00042734903,0.00055534014,0.0010379431,0.0005882056,0.0008533664,0.0003341572,0.00018229062],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017192154,0.00007091709,0.14172505,0.000021568389,0.00004719931,0.00021772603,0.00023076244,0.8452037,0.0019560168,0.008401026,0.00027644448,0.0016775512],"study_design_scores_gemma":[0.000041506082,0.00007355448,0.031264316,0.000009263458,0.000022030705,0.00010115913,0.00011277348,0.9621095,0.0008563509,0.005015954,0.00037047014,0.000023063618],"about_ca_topic_score_codex":0.025942389,"about_ca_topic_score_gemma":0.016701572,"teacher_disagreement_score":0.025942389,"about_ca_system_score_codex":0.0016117165,"about_ca_system_score_gemma":0.00061469135,"threshold_uncertainty_score":0.051582754},"labels":[],"label_agreement":null},{"id":"W1967756275","doi":"10.1088/0004-637x/775/1/17","title":"STEADY STATE DUST DISTRIBUTIONS IN DISK VORTICES: OBSERVATIONAL PREDICTIONS AND APPLICATIONS TO TRANSITIONAL DISKS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":150,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Vortex; Instability; Rossby wave; Drag; Steady state (chemistry); Millimeter; Diffusion; Dissipative system; Range (aeronautics)","score_opus":0.02122787208604549,"score_gpt":0.25847726342410005,"score_spread":0.23724939133805456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967756275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99658185,0.00008984092,0.0027650227,0.00005901933,0.0000020796688,0.0000065134127,0.00004624116,0.000030435007,0.00041900354],"genre_scores_gemma":[0.99958056,0.000025222254,0.00035087302,0.0000016703061,0.0000024100766,0.000001925856,0.000020717387,0.0000019286128,0.000014798693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989176,0.000027869926,0.000009670669,0.000031724874,0.000016365551,0.000022614784],"domain_scores_gemma":[0.998667,0.0006527527,0.00030826297,0.000132688,0.00015054029,0.000088695444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062773377,0.00027339853,0.0002768668,0.0009477956,0.0005700342,0.0010196058,0.00077111984,0.000642586,0.00032496027],"category_scores_gemma":[0.004536601,0.00031823764,0.00040039327,0.00047392905,0.0011163789,0.0010256515,0.0007221757,0.00036678844,0.00006570167],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040962576,0.00027132616,0.797074,0.00012590841,0.00007977461,0.00072437944,0.0011948824,0.14221543,0.022444649,0.01899867,0.00038315685,0.016078223],"study_design_scores_gemma":[0.00008869122,0.000090648165,0.19803938,0.00003348616,0.000027164977,0.00020156297,0.00063481973,0.781712,0.005421893,0.0133626005,0.0003294144,0.000058256832],"about_ca_topic_score_codex":0.0074152807,"about_ca_topic_score_gemma":0.0030316373,"teacher_disagreement_score":0.0074152807,"about_ca_system_score_codex":0.001137112,"about_ca_system_score_gemma":0.00028554027,"threshold_uncertainty_score":0.014744282},"labels":[],"label_agreement":null},{"id":"W1967785029","doi":"10.1088/0004-637x/786/2/115","title":"<i>RADIOASTRON</i>STUDIES OF THE NEARBY, TURBULENT INTERSTELLAR PLASMA WITH THE LONGEST SPACE-GROUND INTERFEROMETER BASELINE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Scintillation; Pulsar; Very Long Baseline Array; Telescope; Radio telescope; Interstellar medium; Very-long-baseline interferometry; Interferometry; Spectral line","score_opus":0.014788740579302302,"score_gpt":0.2819475237612335,"score_spread":0.2671587831819312,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967785029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991048,0.00007133391,0.00022501689,0.0000074861127,0.0000011231326,0.0000015674187,0.00007235926,0.000008911964,0.0005073915],"genre_scores_gemma":[0.9993711,0.00004012825,0.00028410516,0.000005128941,0.0000033862134,0.0000020319555,0.00022019389,0.000002513379,0.00007146337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999614,0.0000048363236,0.0000023583063,0.000010402042,0.000011708767,0.000009301478],"domain_scores_gemma":[0.99981076,0.000024770845,0.00008699296,0.000014261212,0.00002610802,0.00003715978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013456686,0.000097299315,0.00007942776,0.00062604377,0.0002612613,0.00028177176,0.00011676659,0.00009461434,0.0003024023],"category_scores_gemma":[0.00025303932,0.0000746522,0.00010954911,0.000583164,0.00022277993,0.00014976384,0.00019664879,0.00009906522,0.00006162627],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030809984,0.00005046624,0.82276523,0.0000404498,0.00008305612,0.00059972,0.00046157185,0.0020119278,0.16148135,0.0007044255,0.00030657309,0.01118707],"study_design_scores_gemma":[0.000004440547,0.000056152807,0.99598724,0.0000019533422,0.000008451232,0.000162664,0.000049223654,0.00090244925,0.0023464556,0.00008074938,0.00039652895,0.000003692901],"about_ca_topic_score_codex":0.0015852774,"about_ca_topic_score_gemma":0.0033115114,"teacher_disagreement_score":0.0015852774,"about_ca_system_score_codex":0.00021831905,"about_ca_system_score_gemma":0.00009243197,"threshold_uncertainty_score":0.003152132},"labels":[],"label_agreement":null},{"id":"W1967786223","doi":"10.1086/312816","title":"Temperature and Density Gradients Across the Nucleus of M82","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"James Clerk Maxwell Telescope; Line (geometry); Torus; Galaxy; Spectral line; Density gradient; Star formation; Temperature gradient; Active galactic nucleus","score_opus":0.004384831550205215,"score_gpt":0.2064269902952749,"score_spread":0.20204215874506967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967786223","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993813,0.000035056022,0.00004474793,0.00001356001,6.730887e-7,4.6129207e-7,0.00005672735,0.0000065286144,0.00046077222],"genre_scores_gemma":[0.9996729,0.000017050823,0.000045388064,0.0000074874483,0.0000021262845,0.000001120158,0.00008301405,0.0000028198663,0.00016815997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999511,0.0000036220777,0.0000018783782,0.000018291847,0.000010589761,0.0000144409405],"domain_scores_gemma":[0.9998654,0.000012937927,0.00004003561,0.0000127536305,0.000039935814,0.000028859567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000047069167,0.00009803338,0.00014424886,0.00045379586,0.000221027,0.0003459512,0.00014088779,0.00019593496,0.00066256354],"category_scores_gemma":[0.0002722187,0.00014396688,0.00007369633,0.0002307891,0.00019361611,0.00019103198,0.00032608025,0.0001197387,0.00023971155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034275232,0.000034376433,0.7030009,0.000027079403,0.000057498306,0.00048235437,0.0011000055,0.000918145,0.28509572,0.0002857509,0.00040203557,0.008253406],"study_design_scores_gemma":[0.0000023995199,0.000012597622,0.9979546,0.0000013628248,0.0000041826383,0.00006307311,0.00011394736,0.00030374204,0.0013188442,0.000024586905,0.00019798242,0.0000027209371],"about_ca_topic_score_codex":0.0066271666,"about_ca_topic_score_gemma":0.009336601,"teacher_disagreement_score":0.0066271666,"about_ca_system_score_codex":0.00030203638,"about_ca_system_score_gemma":0.00007995645,"threshold_uncertainty_score":0.013177216},"labels":[],"label_agreement":null},{"id":"W1967821305","doi":"10.1088/0004-637x/713/1/710","title":"ERRATUM: “A PRECISE MASS MEASUREMENT OF THE INTERMEDIATE-MASS BINARY PULSAR PSR J1802–2124” (2010, ApJ, 711, 764)","year":2010,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Geophysics and Gravity Measurements","field":"Earth and Planetary Sciences","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Pulsar; Binary number; Astrophysics; Astronomy; Arithmetic","score_opus":0.02034744780218082,"score_gpt":0.2122099617105911,"score_spread":0.19186251390841028,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967821305","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0015904283,0.0017218802,0.0012145076,0.0368196,0.94568413,0.00003473944,0.0033268034,0.0008079007,0.008800023],"genre_scores_gemma":[0.06464671,0.01496186,0.016664745,0.11676726,0.21853313,0.00038913713,0.027888091,0.004790097,0.53535897],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99817896,0.00018825318,0.00038439294,0.00024121338,0.0008852103,0.00012209386],"domain_scores_gemma":[0.99153614,0.0012788615,0.0007669164,0.0007062841,0.005312992,0.000398885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014691036,0.0023588357,0.0012142811,0.0029408406,0.004164448,0.0021856294,0.0018943894,0.0042873,0.03272752],"category_scores_gemma":[0.018206287,0.0010817683,0.0010485587,0.0021237512,0.0015283383,0.0021788753,0.00172692,0.006149418,0.04746688],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000070098715,0.000017306062,0.0003015295,0.000104429455,0.000011349398,0.00030185923,0.000035380875,0.000056086836,0.00022615759,0.00072736765,0.98949,0.00865848],"study_design_scores_gemma":[0.000052172694,0.00007332228,0.0040305248,0.00027492933,0.00005219927,0.0008802846,0.00014612754,0.00030970803,0.0014945127,0.0010579439,0.99155504,0.00007326916],"about_ca_topic_score_codex":0.01728525,"about_ca_topic_score_gemma":0.018647116,"teacher_disagreement_score":0.03272752,"about_ca_system_score_codex":0.0027508484,"about_ca_system_score_gemma":0.0031893798,"threshold_uncertainty_score":0.109484434},"labels":[],"label_agreement":null},{"id":"W1967828416","doi":"10.1086/507327","title":"Discovery of Carbon/Oxygen-depleted Blue Straggler Stars in 47 Tucanae: The Chemical Signature of a Mass Transfer Formation Process","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Blue straggler; Stars; Mass transfer; Process (computing); Carbon fibers; Chemistry; Astrophysics; Globular cluster; Physics; Computer science; Chromatography; Algorithm","score_opus":0.005397397965780644,"score_gpt":0.1984573572695906,"score_spread":0.19305995930380995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967828416","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997466,0.000023036153,0.00002854597,0.00000365333,5.411264e-7,0.0000012519279,0.00003931556,0.0000033538686,0.00015360607],"genre_scores_gemma":[0.99948955,0.000030660405,0.00011377857,0.0000057787915,0.0000016383409,0.0000018863304,0.0001772559,0.0000023108605,0.00017705164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990284,0.0000033426156,0.000003209486,0.000019498873,0.000027828855,0.000043342654],"domain_scores_gemma":[0.9998398,0.0000108853665,0.000034154164,0.000014614262,0.00004206831,0.000058469595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001125493,0.0002154624,0.0003211085,0.0013257886,0.0008565832,0.00062750134,0.0003454488,0.00039314284,0.00077769015],"category_scores_gemma":[0.00026356478,0.00013449887,0.00013346328,0.0009159436,0.00048968836,0.0002046776,0.00043046186,0.00019000217,0.00014899085],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027866897,0.000054411474,0.8435007,0.000026331902,0.00007338565,0.0006013739,0.0010919342,0.00039391362,0.14265819,0.00014767148,0.00014330074,0.0110302325],"study_design_scores_gemma":[0.00000465186,0.000036679365,0.9938788,0.0000018482286,0.00001896762,0.00018047466,0.00036173174,0.00039751615,0.0046080216,0.000033609445,0.0004729521,0.000004834236],"about_ca_topic_score_codex":0.07005834,"about_ca_topic_score_gemma":0.093631424,"teacher_disagreement_score":0.07005834,"about_ca_system_score_codex":0.00064837513,"about_ca_system_score_gemma":0.0005217512,"threshold_uncertainty_score":0.13930112},"labels":[],"label_agreement":null},{"id":"W1967905366","doi":"10.1088/0004-637x/755/2/151","title":"A<i>CHANDRA</i>PROPER MOTION FOR PSR J1809–2332","year":2012,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Proper motion; Pulsar wind nebula; Egret; Point source; Supernova remnant; Nebula; Supernova","score_opus":0.02412549092605727,"score_gpt":0.33187992787872417,"score_spread":0.3077544369526669,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967905366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98744327,0.0005173393,0.0017086562,0.00016477321,0.00007562754,0.00003707767,0.002534131,0.0003396902,0.00717949],"genre_scores_gemma":[0.9881974,0.00022058062,0.0056631453,0.00010129348,0.00012117763,0.000029122712,0.0045438455,0.00008961517,0.0010338362],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998441,0.000008344354,0.000007211113,0.000041581592,0.000058811544,0.000039901275],"domain_scores_gemma":[0.9995353,0.000022040727,0.00014346479,0.00008654959,0.00006965965,0.00014299694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023022141,0.0003209821,0.00024034227,0.0013711596,0.0005649463,0.00070074515,0.00035849595,0.00022069135,0.001234775],"category_scores_gemma":[0.0005054807,0.00021662375,0.00028750848,0.0007670782,0.00023101672,0.0004014196,0.00068671507,0.00049868465,0.0005851413],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012053178,0.0004207444,0.41115353,0.00025627503,0.00036964752,0.003357432,0.00076940935,0.001323505,0.4944019,0.0012810307,0.0119803725,0.07348083],"study_design_scores_gemma":[0.000027707993,0.0001643821,0.97038114,0.000011696229,0.00006551402,0.0017685262,0.00007749695,0.0008972464,0.014548395,0.00020471816,0.01180605,0.000047111087],"about_ca_topic_score_codex":0.0038217194,"about_ca_topic_score_gemma":0.008810455,"teacher_disagreement_score":0.0038217194,"about_ca_system_score_codex":0.0002504321,"about_ca_system_score_gemma":0.00029865722,"threshold_uncertainty_score":0.007598996},"labels":[],"label_agreement":null},{"id":"W1967990724","doi":"10.1088/0004-637x/751/2/137","title":"THE SMALL-SCALE PHYSICAL STRUCTURE AND FRAGMENTATION DIFFERENCE OF TWO EMBEDDED INTERMEDIATE-MASS PROTOSTARS IN ORION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Physics; Astrophysics; Fragmentation (computing); Submillimeter Array; Stars; Star formation","score_opus":0.008541463211966227,"score_gpt":0.25645453307970034,"score_spread":0.24791306986773412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1967990724","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998412,0.000014391896,0.000019394321,0.0000024583644,1.9687378e-7,4.8546485e-7,0.000017784385,0.0000018166751,0.00010220377],"genre_scores_gemma":[0.99973303,0.000013719354,0.00008410441,0.0000042490483,9.5280603e-7,0.0000017315627,0.00010686341,0.0000014152848,0.00005394409],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995005,0.0000036288852,0.0000026818575,0.00002091993,0.000008289934,0.000014412239],"domain_scores_gemma":[0.99972266,0.00004184221,0.00011421294,0.000021432243,0.00002366916,0.000076179655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009634906,0.00013191877,0.00015169548,0.0006018973,0.00038040947,0.0003788556,0.00020176628,0.00021248116,0.00047236815],"category_scores_gemma":[0.00030363994,0.00012054108,0.000119335076,0.00038257302,0.00035043777,0.00024445832,0.00039236987,0.000169223,0.00010142894],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031783743,0.00008118404,0.9031447,0.000029399826,0.000027417034,0.0004523798,0.00097378076,0.00067698583,0.0874873,0.00020847113,0.000087207474,0.0065133036],"study_design_scores_gemma":[0.0000022596334,0.000020113408,0.99797386,0.000001844618,0.000003911855,0.000095555726,0.00016736743,0.0005040514,0.0011279156,0.00002457472,0.00007657066,0.0000019155439],"about_ca_topic_score_codex":0.002947083,"about_ca_topic_score_gemma":0.0035255775,"teacher_disagreement_score":0.002947083,"about_ca_system_score_codex":0.00029901508,"about_ca_system_score_gemma":0.00009162242,"threshold_uncertainty_score":0.005859852},"labels":[],"label_agreement":null},{"id":"W1968113693","doi":"10.1086/527296","title":"Clues to the Origin of the Mass-Metallicity Relation: Dependence on Star Formation Rate and Galaxy Size","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":337,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Trent University; University of Victoria","funders":"","keywords":"Galaxy; Star formation; Sky; Stellar mass; Galaxy formation and evolution; Luminous infrared galaxy; Extragalactic astronomy; Elliptical galaxy","score_opus":0.009604511027701145,"score_gpt":0.22662800912453507,"score_spread":0.2170234980968339,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968113693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990018,0.00015356441,0.00020227768,0.000028967546,7.613314e-7,0.0000023798202,0.00023306986,0.000009511676,0.0003676764],"genre_scores_gemma":[0.99943393,0.00004750541,0.000117446245,0.000009523597,0.0000024548847,0.0000015476417,0.000281784,0.000004512099,0.00010112716],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996587,0.00011975978,0.000025027311,0.000087373555,0.00005741558,0.000051716197],"domain_scores_gemma":[0.99465746,0.0023849723,0.0016694994,0.00053331634,0.00030844987,0.0004463249],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00085254596,0.0002574032,0.00041801992,0.0013316738,0.00028060263,0.0006582324,0.00034124462,0.0002985021,0.0013221004],"category_scores_gemma":[0.0038212056,0.0001959557,0.00027010473,0.0012515414,0.00061370846,0.00047705878,0.0005274573,0.00023497087,0.0003490063],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003536958,0.0000068877453,0.997227,0.0000042275583,0.00002602161,0.000024455228,0.000065618515,0.00010441502,0.0014791867,0.000049459235,0.000025024761,0.0009522359],"study_design_scores_gemma":[0.0000016331039,0.000015097284,0.99932826,0.00000121415,0.000008632341,0.000047252477,0.000033812616,0.0002523161,0.00019298242,0.00004517131,0.000072176175,0.0000014426048],"about_ca_topic_score_codex":0.004039148,"about_ca_topic_score_gemma":0.005770135,"teacher_disagreement_score":0.004039148,"about_ca_system_score_codex":0.00021392874,"about_ca_system_score_gemma":0.00014343606,"threshold_uncertainty_score":0.008031249},"labels":[],"label_agreement":null},{"id":"W1968168059","doi":"10.1086/504822","title":"O<scp>vi</scp>Asymmetry and an Accelerated Outflow in an Obscured Seyfert:<i>FUSE</i>and<i>HST</i>STIS Spectroscopy of Mrk 533","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Outflow; Physics; Astrophysics; Spectral line; Asymmetry; Galaxy; Wavelength; Fuse (electrical); Emission spectrum; Spectroscopy; Ionization; Line (geometry); Optics; Astronomy; Geometry; Meteorology","score_opus":0.008267834575282455,"score_gpt":0.22932270125075707,"score_spread":0.2210548666754746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968168059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960731,0.00008961745,0.00013491718,0.00026638684,0.000029460713,0.000009733428,0.00024597172,0.00003133619,0.0031194114],"genre_scores_gemma":[0.9990206,0.000024599205,0.00008991256,0.000071265276,0.00005341285,0.0000017878791,0.00014565815,0.000010763069,0.0005820828],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999362,0.0000036188644,0.000005999679,0.000016407834,0.000016295262,0.000021408892],"domain_scores_gemma":[0.99943906,0.00009215422,0.00014428735,0.000041745934,0.00009003708,0.00019270256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020983447,0.00029448,0.0003009628,0.00073243736,0.0005391411,0.00047488164,0.00040293572,0.0008425821,0.005097685],"category_scores_gemma":[0.0006685538,0.00016985639,0.0001937116,0.00036690998,0.0003967794,0.00040807095,0.00032445256,0.00047963613,0.00075808074],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004581778,0.0006351214,0.69905096,0.000102650294,0.00014030965,0.09348253,0.0011860783,0.00057386566,0.17534342,0.00075917115,0.0066751055,0.017468978],"study_design_scores_gemma":[0.000072431474,0.00029575144,0.97843194,0.000009474729,0.000043915366,0.014242542,0.00024318826,0.00076778914,0.0045284075,0.0001730884,0.0011771863,0.000014222195],"about_ca_topic_score_codex":0.0055432445,"about_ca_topic_score_gemma":0.004678015,"teacher_disagreement_score":0.0055432445,"about_ca_system_score_codex":0.000238256,"about_ca_system_score_gemma":0.00017845073,"threshold_uncertainty_score":0.017053485},"labels":[],"label_agreement":null},{"id":"W1968179298","doi":"10.1086/513085","title":"Star Formation at Very Low Metallicity. II. On the Insignificance of Metal‐Line Cooling During the Early Stages of Gravitational Collapse","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Metallicity; Astrophysics; Reionization; Physics; Halo; Star formation; Population; Stars; Gravitational collapse; Galaxy; Redshift","score_opus":0.009562841421083197,"score_gpt":0.21631217017607673,"score_spread":0.20674932875499355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968179298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99884653,0.000037321774,0.00035316512,0.00003966632,0.000002802937,0.0000053599397,0.00006426591,0.000020960531,0.0006298231],"genre_scores_gemma":[0.9994357,0.000030254327,0.00021047845,0.00002240966,0.0000033695646,0.0000049136875,0.000095755764,0.000008663002,0.00018854107],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999118,0.000018012599,0.000003484776,0.000016995797,0.000012012683,0.00003774269],"domain_scores_gemma":[0.9994186,0.00016843752,0.00013808478,0.000045497454,0.000042075742,0.00018734038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002512311,0.00038204854,0.00036479815,0.0002898929,0.00039876768,0.00086592697,0.00048657443,0.00064071716,0.001160319],"category_scores_gemma":[0.0015223767,0.00021371427,0.0004639443,0.00019691541,0.00077368564,0.00043116417,0.00064051594,0.00054266397,0.00023485665],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014956235,0.00048568356,0.3843733,0.00026631771,0.00040171994,0.0017425555,0.0007446477,0.49528158,0.09719539,0.008568051,0.0012392871,0.008205892],"study_design_scores_gemma":[0.00042704743,0.0009161405,0.2662368,0.000037131285,0.00014497612,0.0003402593,0.0005180518,0.7079583,0.014923517,0.006954784,0.0014785096,0.00006456744],"about_ca_topic_score_codex":0.005381688,"about_ca_topic_score_gemma":0.0048781717,"teacher_disagreement_score":0.005381688,"about_ca_system_score_codex":0.0006163389,"about_ca_system_score_gemma":0.00029066697,"threshold_uncertainty_score":0.010700703},"labels":[],"label_agreement":null},{"id":"W1968193817","doi":"10.1088/0004-637x/783/1/3","title":"THE ORBITS OF THE TRIPLE-STAR SYSTEM 1 GEMINORUM FROM PHASES DIFFERENTIAL ASTROMETRY AND SPECTROSCOPY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrometry; Astrophysics; Astronomy; Spectroscopy; Star (game theory); Differential (mechanical device); Stars","score_opus":0.0062324545493589395,"score_gpt":0.20682777198329816,"score_spread":0.2005953174339392,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968193817","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957747,0.00019854777,0.0011975475,0.000033258657,0.000009891788,0.000009554745,0.0002178355,0.000027850785,0.0025309613],"genre_scores_gemma":[0.9966486,0.00005348974,0.0022535848,0.000011242049,0.0000066463663,0.0000052345645,0.0006898811,0.000012258651,0.00031902577],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998603,0.000022122347,0.0000089666155,0.00004400058,0.00004278945,0.000021838607],"domain_scores_gemma":[0.9997199,0.000024713669,0.00010940065,0.000039545997,0.000048797217,0.000057603324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003247255,0.00021620901,0.00024429755,0.0009414671,0.0005689296,0.00063664035,0.00021716206,0.0002691936,0.0012168863],"category_scores_gemma":[0.00049597357,0.00016163486,0.0001583367,0.00066316343,0.00024448909,0.00035040386,0.0007663351,0.00034945243,0.0004162327],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013553059,0.0001244303,0.5093954,0.00030114243,0.00014015635,0.0006976424,0.0022662214,0.005348936,0.36811316,0.009788795,0.0017648138,0.1007039],"study_design_scores_gemma":[0.00006716125,0.00095563906,0.89168656,0.00010299369,0.00014708041,0.002043643,0.0010645005,0.028340762,0.04699766,0.0065787286,0.021936247,0.00007912435],"about_ca_topic_score_codex":0.00094895123,"about_ca_topic_score_gemma":0.002338205,"teacher_disagreement_score":0.0012168863,"about_ca_system_score_codex":0.00031299188,"about_ca_system_score_gemma":0.0002506263,"threshold_uncertainty_score":0.004070878},"labels":[],"label_agreement":null},{"id":"W1968219989","doi":"10.1086/590368","title":"Outflow and Infall in a Sample of Massive Star Forming Regions. II. Large‐Scale Kinematics","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"James Clerk Maxwell Telescope; Outflow; Luminosity; Star formation; Star (game theory); High mass; Entrainment (biomusicology); Scaling","score_opus":0.013507957412519703,"score_gpt":0.23508201018905747,"score_spread":0.22157405277653777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968219989","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99958044,0.000049871764,0.00004653492,0.000007244126,3.927376e-7,0.0000019820852,0.0001471429,0.0000023998907,0.0001640299],"genre_scores_gemma":[0.99877936,0.00006525893,0.00018249315,0.000006768375,0.0000032516916,0.0000034823233,0.00083056715,0.000002387177,0.00012649327],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989176,0.0000149553025,0.00000664049,0.00002623466,0.000017744285,0.00004265321],"domain_scores_gemma":[0.9995371,0.000074323485,0.00020956277,0.000029839392,0.000028873048,0.0001202968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016311764,0.0001922163,0.00017452188,0.0011530212,0.00034503653,0.0003955648,0.0001685002,0.00016791592,0.0007803233],"category_scores_gemma":[0.00053214486,0.0001620812,0.0001663175,0.0007527088,0.00026884733,0.00021999869,0.0006018362,0.0001531607,0.00016256876],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006919913,0.000017712011,0.99329776,0.000007300682,0.00001610556,0.00017763903,0.00036692497,0.00009421614,0.0031909228,0.00004878234,0.00007687285,0.0026366229],"study_design_scores_gemma":[0.0000014575614,0.000014002556,0.99929154,0.0000010028925,0.0000035456849,0.00019216965,0.00013604079,0.00008090988,0.00014853955,0.000014923166,0.00011475958,0.0000010737559],"about_ca_topic_score_codex":0.009248576,"about_ca_topic_score_gemma":0.020334134,"teacher_disagreement_score":0.009248576,"about_ca_system_score_codex":0.00022248253,"about_ca_system_score_gemma":0.00012210215,"threshold_uncertainty_score":0.018389523},"labels":[],"label_agreement":null},{"id":"W1968271641","doi":"10.1086/425974","title":"A QED Model for the Origin of Bursts from Soft Gamma Repeaters and Anomalous X‐Ray Pulsars","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Neutron star; Pulsar; Magnetohydrodynamics; Amplitude; Astrophysics; Magnetic field; Electron; Wavelength; Electromagnetic radiation; Magnetar; Classification of discontinuities; Polarization (electrochemistry); Pair production; Radiative transfer; Quantum electrodynamics; Computational physics; Nuclear physics; Quantum mechanics","score_opus":0.018285956753289676,"score_gpt":0.30567927778698845,"score_spread":0.28739332103369875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968271641","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.48729518,0.0016513532,0.3591818,0.014302336,0.00080428465,0.00020657029,0.00081725186,0.000820841,0.13492037],"genre_scores_gemma":[0.95391357,0.00043211522,0.01523991,0.0006635321,0.00026279705,0.00019726017,0.00016934492,0.00008522249,0.029036311],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99988115,0.000018020672,0.0000058649025,0.000028155424,0.000029880508,0.000036878082],"domain_scores_gemma":[0.9997209,0.00006340059,0.00005338081,0.000038337592,0.000046953388,0.000077022974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034491022,0.0004052934,0.0004984658,0.0005253259,0.0007637576,0.0011535706,0.001942684,0.0014772859,0.006505024],"category_scores_gemma":[0.00064050895,0.00030434565,0.0010613858,0.00033151906,0.0013279693,0.00196471,0.0013621631,0.0010102148,0.0012418075],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007174804,0.000058035992,0.0035658656,0.00005221718,0.000035223813,0.0015558834,0.0004884243,0.09549438,0.009010458,0.8810294,0.002823285,0.005815101],"study_design_scores_gemma":[0.0001460648,0.00008582139,0.0023352548,0.00001650109,0.000019339363,0.0007469405,0.00012549735,0.5547497,0.0005931941,0.43351272,0.007621395,0.00004751038],"about_ca_topic_score_codex":0.0031464277,"about_ca_topic_score_gemma":0.0010234275,"teacher_disagreement_score":0.006505024,"about_ca_system_score_codex":0.0011414553,"about_ca_system_score_gemma":0.0005514764,"threshold_uncertainty_score":0.021761417},"labels":[],"label_agreement":null},{"id":"W1968306279","doi":"10.1086/498691","title":"Reddening Distribution across the Center of the Globular Cluster ω Centauri","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Photometry (optics); Metallicity; Astronomy; Stars; Star cluster; Extinction (optical mineralogy)","score_opus":0.007274152930310192,"score_gpt":0.2335350089031577,"score_spread":0.2262608559728475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968306279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999331,0.00010513436,0.00012963542,0.00000552268,7.9004957e-7,6.1492045e-7,0.00005623729,0.000010888318,0.00036020367],"genre_scores_gemma":[0.99960107,0.000050794693,0.00007990502,0.0000038259423,0.0000023287805,0.0000010447591,0.00013104315,0.0000034601549,0.0001265512],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998759,0.000011428477,0.000006953491,0.000043727054,0.000031633677,0.00003043661],"domain_scores_gemma":[0.99920243,0.00018014084,0.00021468425,0.00011445601,0.00016251416,0.00012593548],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025050805,0.00012940668,0.00019277961,0.0018328294,0.00027984334,0.0004910282,0.00022774583,0.0001606544,0.0011235778],"category_scores_gemma":[0.0010372516,0.00010779918,0.000105699546,0.00076202845,0.0004242876,0.00021846253,0.0006104448,0.000104604806,0.00021010134],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020137192,0.000013682585,0.9552801,0.00002414545,0.000039776365,0.00015460997,0.0011242062,0.00080979324,0.019767422,0.00041497627,0.00028875555,0.021881122],"study_design_scores_gemma":[0.0000015448574,0.000018679668,0.9985877,0.000004038752,0.000009481267,0.00012341086,0.00010662927,0.0003172548,0.0004713902,0.000082931285,0.00027328372,0.0000035457165],"about_ca_topic_score_codex":0.0066451123,"about_ca_topic_score_gemma":0.007920859,"teacher_disagreement_score":0.0066451123,"about_ca_system_score_codex":0.00038416646,"about_ca_system_score_gemma":0.000081893624,"threshold_uncertainty_score":0.01321286},"labels":[],"label_agreement":null},{"id":"W1968360036","doi":"10.1088/0004-637x/740/2/65","title":"A VERY LARGE ARRAY SEARCH FOR 5 GHz RADIO TRANSIENTS AND VARIABLES AT LOW GALACTIC LATITUDES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Sky; Astrophysics; Jansky; Radio telescope; Latitude; Telescope; Flux (metallurgy); Neutron star; Stars; Astronomy; Galaxy","score_opus":0.015416620699571136,"score_gpt":0.22492682385237528,"score_spread":0.20951020315280414,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968360036","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99044913,0.00027247908,0.005783478,0.00004779843,0.0000085613065,0.000016265945,0.0010000223,0.0001349034,0.002287269],"genre_scores_gemma":[0.99228525,0.00007215826,0.0051675704,0.00003460828,0.000022849843,0.000015435106,0.0018152302,0.000009923214,0.00057699945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997887,0.0000440389,0.000009451767,0.00008001413,0.000032926037,0.000044939665],"domain_scores_gemma":[0.99959546,0.00011300432,0.0001055779,0.000044918426,0.000038369653,0.00010268133],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000353815,0.00014701569,0.00021301425,0.001046654,0.00026374427,0.0004545156,0.0002167986,0.00021770938,0.0016644995],"category_scores_gemma":[0.00050537876,0.00012053315,0.00021538557,0.0007484986,0.00007680697,0.00028202494,0.00031513453,0.00014000351,0.00035159444],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038992462,0.000104710256,0.85741884,0.00006611517,0.00012419195,0.00043007193,0.00034549375,0.002125507,0.06158601,0.0010206609,0.0018745766,0.07451394],"study_design_scores_gemma":[0.000021647758,0.00017799261,0.9920322,0.000009293801,0.00005211115,0.0002837822,0.00012570656,0.0021963376,0.0021977667,0.00021228842,0.00268038,0.0000106091375],"about_ca_topic_score_codex":0.00094974943,"about_ca_topic_score_gemma":0.0019902778,"teacher_disagreement_score":0.0016644995,"about_ca_system_score_codex":0.000110115296,"about_ca_system_score_gemma":0.00011449953,"threshold_uncertainty_score":0.005568266},"labels":[],"label_agreement":null},{"id":"W1968384442","doi":"10.1088/0004-637x/696/2/1461","title":"SPECTROSCOPIC ANALYSIS OF THE WHITE DWARF KUV 02196+2816: A NEW UNRESOLVED DA+DB DEGENERATE BINARY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"White dwarf; Chandrasekhar limit; Physics; Astrophysics; Degenerate energy levels; Helium; Stars; Spectral line; Line (geometry); Effective temperature; Stellar classification; Star (game theory); Astronomy; Atomic physics; Mathematics","score_opus":0.012825010174267697,"score_gpt":0.2379425866449662,"score_spread":0.2251175764706985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968384442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992949,0.00009822083,0.000073311036,0.000009097219,0.0000035618561,0.0000040682253,0.0000791635,0.000005055124,0.00043270967],"genre_scores_gemma":[0.99864835,0.00005501747,0.0003627249,0.000011795673,0.000007614581,0.000003927722,0.00048715572,0.0000033617507,0.00042006723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998827,0.000007465182,0.000012058487,0.00004333674,0.000034090674,0.000020413003],"domain_scores_gemma":[0.99972945,0.000014696419,0.000080109094,0.000028523382,0.000026465998,0.00012071785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010497763,0.00041740673,0.00047688527,0.0012669064,0.000688694,0.00048073876,0.00045663983,0.00037681314,0.0008189189],"category_scores_gemma":[0.00024558412,0.00021634223,0.00014425423,0.00093056564,0.00038714087,0.00019464863,0.0005800533,0.00023445749,0.0004990244],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009379698,0.00039341688,0.59110975,0.00015484245,0.00008518865,0.0058382177,0.0006439711,0.0004895643,0.37347448,0.0006314635,0.00034144212,0.025899652],"study_design_scores_gemma":[0.00005860317,0.0010452224,0.9566384,0.000017563978,0.000054874163,0.014441707,0.00048740229,0.0012959675,0.020004952,0.00038832703,0.0055424008,0.000024637342],"about_ca_topic_score_codex":0.0010475647,"about_ca_topic_score_gemma":0.0015480792,"teacher_disagreement_score":0.0012669064,"about_ca_system_score_codex":0.00033674343,"about_ca_system_score_gemma":0.00013471629,"threshold_uncertainty_score":0.0027395487},"labels":[],"label_agreement":null},{"id":"W1968389390","doi":"10.1088/0004-637x/747/1/44","title":"THE 15–20 μm EMISSION IN THE REFLECTION NEBULA NGC 2023","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Reflection nebula; Physics; Astrophysics; Nebula; Spitzer Space Telescope; Emission spectrum; Spectral resolution; Spectral energy distribution; Spectrograph; Infrared; Spectral line; Astronomy; Galaxy; Stars","score_opus":0.01743436117501022,"score_gpt":0.28174076715689517,"score_spread":0.26430640598188493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968389390","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944729,0.00016047702,0.00048127593,0.000043716194,0.000002414669,0.000004028471,0.00036705457,0.00021500143,0.0042531695],"genre_scores_gemma":[0.9979424,0.00006644857,0.0007286226,0.000036570164,0.000004772922,0.000006808149,0.0006580225,0.00002450942,0.00053192605],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999571,0.0000024220094,0.0000013500968,0.0000114747945,0.000010922543,0.000016698212],"domain_scores_gemma":[0.99994135,0.0000046431055,0.000021839796,0.0000041458225,0.000007511784,0.0000205488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007191264,0.00022547308,0.00012864449,0.00044691202,0.00026935455,0.00023969807,0.00024245119,0.00024244054,0.0017902358],"category_scores_gemma":[0.000074298165,0.00014430966,0.00025848727,0.00031499664,0.00019311813,0.00012640453,0.00022292037,0.00019658635,0.0005605537],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003681967,0.000096765616,0.30580583,0.00011579549,0.000091632704,0.0011809056,0.0007500053,0.0017964124,0.6607212,0.00059765537,0.0016725681,0.026803058],"study_design_scores_gemma":[0.000010072355,0.00004364192,0.9897857,0.000008459816,0.000018094157,0.0003744142,0.00011388493,0.001258988,0.006447285,0.00012175973,0.0018102147,0.0000074975696],"about_ca_topic_score_codex":0.0071549835,"about_ca_topic_score_gemma":0.009990402,"teacher_disagreement_score":0.0071549835,"about_ca_system_score_codex":0.0004342071,"about_ca_system_score_gemma":0.000168879,"threshold_uncertainty_score":0.014226675},"labels":[],"label_agreement":null},{"id":"W1968411032","doi":"10.1086/526449","title":"Search for Mid‐Infrared Flux Variations from the Anomalous X‐Ray Pulsar 4U 0142+61","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Infrared; Flux (metallurgy); Astrophysics; X-ray pulsar; Astronomy; Materials science","score_opus":0.02196070930370978,"score_gpt":0.3053345372332035,"score_spread":0.28337382792949367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968411032","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991817,0.00013598798,0.00011104954,0.000021986856,0.000004054036,0.0000035025214,0.00003535499,0.000007574737,0.0004988885],"genre_scores_gemma":[0.99835867,0.00019869636,0.00070354686,0.00004718561,0.000038650116,0.000010220733,0.00035534633,0.00000552861,0.00028218774],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986804,0.000014218423,0.000008623251,0.00003393208,0.000044201828,0.000031042327],"domain_scores_gemma":[0.99957055,0.000055777375,0.00020314757,0.000043331722,0.000044762764,0.00008239746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028204024,0.00023500719,0.00032432668,0.0011671743,0.0005538825,0.00054510124,0.00030629593,0.0004614853,0.000678971],"category_scores_gemma":[0.00046007402,0.00024125072,0.0001826069,0.0006427412,0.00024687836,0.00033887767,0.00064022915,0.00042254615,0.0002340037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026555939,0.00015454293,0.8526066,0.000063419815,0.000092121416,0.0016876425,0.00060337316,0.00032745174,0.117822535,0.00025502112,0.00043961665,0.0256822],"study_design_scores_gemma":[0.00000954574,0.00019839902,0.99459994,0.0000057231055,0.000026110602,0.0007781623,0.00014616895,0.0003409283,0.0027548329,0.00010429321,0.0010287473,0.000007134049],"about_ca_topic_score_codex":0.00041037492,"about_ca_topic_score_gemma":0.0011336716,"teacher_disagreement_score":0.0011671743,"about_ca_system_score_codex":0.00009855593,"about_ca_system_score_gemma":0.00012112456,"threshold_uncertainty_score":0.0022713542},"labels":[],"label_agreement":null},{"id":"W1968498362","doi":"10.1086/588657","title":"The Ionization of Accretion Flows in High-Mass Star Formation: W51e2","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Accretion (finance); Outflow; Ionization; Bipolar outflow; Line (geometry); Angular resolution (graph drawing); Velocity gradient; Star formation; Intermediate polar","score_opus":0.009991197052900724,"score_gpt":0.21792895081000885,"score_spread":0.20793775375710813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968498362","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99928325,0.000038389688,0.00006783285,0.000007854118,8.1789034e-7,0.000002012264,0.00002157407,0.000002719643,0.0005754896],"genre_scores_gemma":[0.99954635,0.00002190351,0.00007353383,0.0000075344965,0.0000023339358,0.000002617027,0.000111692614,0.0000021845442,0.00023184426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994564,0.0000054166194,0.0000035939015,0.000013663195,0.000010121942,0.000021596814],"domain_scores_gemma":[0.99991536,0.000010452087,0.000024814794,0.000005763082,0.000010014835,0.000033620297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014982584,0.0001874123,0.00016111169,0.00046246953,0.0004124404,0.0006452005,0.00016058548,0.00023807069,0.0008377587],"category_scores_gemma":[0.0003337621,0.00016671048,0.000105954256,0.00026162673,0.0002837386,0.0003277511,0.0004954417,0.00020820266,0.00021925404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009719963,0.00019207828,0.67392594,0.000054471082,0.0000847302,0.0025861925,0.00084050104,0.001051739,0.30729505,0.0013358432,0.00050369644,0.01115771],"study_design_scores_gemma":[0.00003594583,0.00007811708,0.99002635,0.0000053795147,0.000010217584,0.0009007575,0.0001489345,0.0013933096,0.0065663946,0.00024818713,0.00058116135,0.000005298417],"about_ca_topic_score_codex":0.0022822786,"about_ca_topic_score_gemma":0.0025735458,"teacher_disagreement_score":0.0022822786,"about_ca_system_score_codex":0.00030781055,"about_ca_system_score_gemma":0.00012192217,"threshold_uncertainty_score":0.00453794},"labels":[],"label_agreement":null},{"id":"W1968584055","doi":"10.1086/431964","title":"On the Relevance of the Tremaine‐Weinberg Method Applied to an Hα Velocity Field: Pattern Speed Determination in M100 (NGC 4321)","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Spiral galaxy; Galaxy; Bar (unit); Halo; Vector field; Field (mathematics); Virgo Cluster; Spiral (railway); Galaxy cluster; Mechanics","score_opus":0.00883863421001797,"score_gpt":0.24706757367568727,"score_spread":0.2382289394656693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968584055","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7866063,0.00013374523,0.20961986,0.00008854616,0.000028883363,0.00006835144,0.000149174,0.0004220037,0.0028830552],"genre_scores_gemma":[0.9265877,0.00007684612,0.07253173,0.000017343875,0.000009896757,0.00005161143,0.00010349042,0.00004322264,0.00057817524],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99902344,0.00046672075,0.00005141413,0.0002104498,0.00018764692,0.000060199847],"domain_scores_gemma":[0.991751,0.005025361,0.0011300164,0.0010633679,0.00081215246,0.00021820444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029230942,0.00036490458,0.0002803577,0.0012506905,0.00039041476,0.0007790539,0.0009821141,0.00048523882,0.0007919812],"category_scores_gemma":[0.01632513,0.00021676013,0.00023468921,0.00068183715,0.00065598736,0.0008367714,0.00070324994,0.00037143784,0.0004344938],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067829614,0.00017667079,0.45719832,0.0001789725,0.00018953322,0.0005402585,0.00060903456,0.22640355,0.035488848,0.016067984,0.0006305158,0.26183802],"study_design_scores_gemma":[0.000039775754,0.0002185517,0.06105204,0.000020517064,0.000028192215,0.0004203327,0.00012215138,0.90795654,0.024176331,0.0052967216,0.00061331526,0.000055470508],"about_ca_topic_score_codex":0.0046658865,"about_ca_topic_score_gemma":0.003933785,"teacher_disagreement_score":0.0046658865,"about_ca_system_score_codex":0.0004918365,"about_ca_system_score_gemma":0.0006174375,"threshold_uncertainty_score":0.015459001},"labels":[],"label_agreement":null},{"id":"W1968675256","doi":"10.1088/0004-637x/729/2/146","title":"EMBEDDED PROTOSTELLAR DISKS AROUND (SUB-)SOLAR STARS. II. DISK MASSES, SIZES, DENSITIES, TEMPERATURES, AND THE PLANET FORMATION PERSPECTIVE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Planet; Protostar; Stars; Gravitational instability; Accretion (finance); Millimeter; Debris disk; Gravitation; Protoplanetary disk; Star formation","score_opus":0.011153582229509343,"score_gpt":0.2192920001393595,"score_spread":0.20813841790985016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968675256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99501604,0.0012216229,0.0019149943,0.00004015767,0.000006570218,0.0000057083694,0.00015779416,0.000016740878,0.0016203703],"genre_scores_gemma":[0.9985727,0.00046983917,0.0006472287,0.0000064691053,0.0000044085136,0.0000021884982,0.000112627175,0.0000043671666,0.00018025476],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999758,0.0000038768458,0.000001634293,0.000008527535,0.00000478189,0.000005352654],"domain_scores_gemma":[0.9998847,0.000028909408,0.000043130218,0.000013914063,0.000010278517,0.000019021787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000043821077,0.00027059705,0.00014258201,0.00019312475,0.00016723412,0.0005259637,0.00033307486,0.00019999973,0.0005958512],"category_scores_gemma":[0.00036565642,0.00012660984,0.00013098045,0.00018920166,0.00026494445,0.00047971567,0.00028435932,0.00016090261,0.0001509423],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029631652,0.00021098532,0.6191478,0.00037756943,0.00017418794,0.0014951907,0.000623543,0.18645859,0.13544147,0.017067216,0.0006898323,0.03801738],"study_design_scores_gemma":[0.00004858924,0.00025426623,0.660546,0.000064028405,0.00008820656,0.0015265812,0.0006815867,0.29107344,0.021698628,0.016785443,0.007203767,0.000029522342],"about_ca_topic_score_codex":0.0016815957,"about_ca_topic_score_gemma":0.0020801804,"teacher_disagreement_score":0.0016815957,"about_ca_system_score_codex":0.00033191752,"about_ca_system_score_gemma":0.00010874023,"threshold_uncertainty_score":0.0033435822},"labels":[],"label_agreement":null},{"id":"W1968816881","doi":"10.1086/527433","title":"A Model for the Total Solar Irradiance Based on Active Region Decay","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université du Québec à Montréal; Université de Montréal","funders":"","keywords":"Sunspot; Irradiance; Physics; Solar irradiance; Brightness; Solar minimum; Astrophysics; Solar maximum; Solar cycle; Atmospheric sciences; Magnetic field; Optics; Solar wind","score_opus":0.02004489898727965,"score_gpt":0.2333707086121715,"score_spread":0.21332580962489184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968816881","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.20261922,0.00057634915,0.7525712,0.001124349,0.0001469424,0.00019681074,0.0027704877,0.0009978551,0.038996723],"genre_scores_gemma":[0.9263975,0.000542239,0.038462106,0.00021821857,0.000085267566,0.0004660367,0.0013576229,0.00039697846,0.032074053],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996105,0.000094357856,0.000016480262,0.00014710551,0.00006278854,0.000068869755],"domain_scores_gemma":[0.9993154,0.00031886605,0.000099960685,0.000061015642,0.00014262652,0.00006218122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006861198,0.0007489003,0.00078942877,0.0006992912,0.000495395,0.0018811615,0.0033199782,0.0023666946,0.007215289],"category_scores_gemma":[0.0024409264,0.0007836049,0.0014731978,0.0011349892,0.0007295906,0.0022235466,0.00064958027,0.0015950083,0.0015100843],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029470766,0.000029878533,0.0016942733,0.00002424118,0.000021346626,0.00007297828,0.00007138462,0.97741187,0.0010851113,0.01557493,0.0008289013,0.0031555586],"study_design_scores_gemma":[0.000013989647,0.000010648031,0.0005643705,0.0000051074076,0.000008611279,0.00003718992,0.000010961683,0.9941632,0.00011145156,0.004206012,0.0008591674,0.000009308198],"about_ca_topic_score_codex":0.02094503,"about_ca_topic_score_gemma":0.012128936,"teacher_disagreement_score":0.02094503,"about_ca_system_score_codex":0.0019596862,"about_ca_system_score_gemma":0.00097389496,"threshold_uncertainty_score":0.041646242},"labels":[],"label_agreement":null},{"id":"W1968853573","doi":"10.1086/308907","title":"New Techniques for Relating Dynamically Close Galaxy Pairs to Merger and Accretion Rates: Application to the Second Southern Sky Redshift Survey","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Statistical Methods and Models","field":"Mathematics","cited_by":250,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Galaxy; Redshift; Luminosity function; Accretion (finance); Galaxy formation and evolution; Redshift survey; Luminosity; Sky; Astronomy; Absolute magnitude; Statistic; Statistics; Mathematics","score_opus":0.03428260319589021,"score_gpt":0.35847634029199865,"score_spread":0.32419373709610844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968853573","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2605937,0.0010178646,0.728948,0.000434375,0.00009621029,0.00018833128,0.0019100329,0.0018490343,0.0049624974],"genre_scores_gemma":[0.76480985,0.00047697738,0.23040779,0.00012425563,0.00020329522,0.00031362067,0.0017031621,0.00041743714,0.0015435597],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.997663,0.0010960522,0.00016636573,0.0003878051,0.0006032333,0.00008350298],"domain_scores_gemma":[0.9806686,0.01135007,0.0037836598,0.0028556366,0.0008821577,0.00045987644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0050948607,0.00078783784,0.0008537165,0.0057355464,0.0006600155,0.0012848055,0.0010326206,0.0005298652,0.0017025191],"category_scores_gemma":[0.030141147,0.00045065762,0.00095186016,0.0044092825,0.0009665521,0.0011574306,0.0019148352,0.0012068944,0.00046693286],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001426889,0.000085676766,0.71245307,0.00021389197,0.0006207672,0.00037698427,0.00089827925,0.05917886,0.007847465,0.040239986,0.0035783583,0.17436394],"study_design_scores_gemma":[0.0000701342,0.00029107824,0.6199726,0.00007802486,0.00019154332,0.0020953678,0.0004588085,0.2971599,0.008312122,0.050876226,0.020153208,0.0003409865],"about_ca_topic_score_codex":0.006725314,"about_ca_topic_score_gemma":0.007324973,"teacher_disagreement_score":0.006725314,"about_ca_system_score_codex":0.0006597092,"about_ca_system_score_gemma":0.0007435963,"threshold_uncertainty_score":0.026944518},"labels":[],"label_agreement":null},{"id":"W1968891632","doi":"10.1088/0004-637x/746/1/105","title":"AN EXTREME PULSAR TAIL PROTRUDING FROM THE FRYING PAN SUPERNOVA REMNANT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Pulsar wind nebula; Supernova remnant; Astrophysics; Astronomy; Nebula; Telescope; Supernova; Stars","score_opus":0.03979146581116887,"score_gpt":0.3260682414931469,"score_spread":0.286276775681978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968891632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99795806,0.00012258421,0.0004499734,0.00001933073,0.000007239414,0.0000062081817,0.00011658544,0.000035260036,0.0012848155],"genre_scores_gemma":[0.9987098,0.000045297613,0.0005550729,0.000021696382,0.000007047601,0.0000020217187,0.00026520708,0.000005651156,0.00038827088],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997246,0.0000016491771,0.0000012550106,0.000009555958,0.0000060965663,0.000008968887],"domain_scores_gemma":[0.9999082,0.0000064621217,0.000035130917,0.000013964188,0.000004470315,0.000031611897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007258894,0.00018394041,0.00017400875,0.00021220258,0.0002846468,0.00024570472,0.00017937722,0.00024105507,0.000882706],"category_scores_gemma":[0.0001736105,0.00007543702,0.0001411422,0.0002161847,0.00022328136,0.00018217266,0.00038639587,0.00027062025,0.00026140606],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009922851,0.00010996481,0.349698,0.00012792152,0.00010285216,0.047499467,0.00040383794,0.00089944183,0.5581895,0.002371209,0.0012612283,0.038344264],"study_design_scores_gemma":[0.000036277655,0.00041374535,0.93265253,0.000017633876,0.000038272614,0.04079595,0.00014183298,0.0010615655,0.017526004,0.0006073671,0.006692366,0.000016269538],"about_ca_topic_score_codex":0.00085828744,"about_ca_topic_score_gemma":0.0011183263,"teacher_disagreement_score":0.000882706,"about_ca_system_score_codex":0.00011188351,"about_ca_system_score_gemma":0.00006297994,"threshold_uncertainty_score":0.002952993},"labels":[],"label_agreement":null},{"id":"W1968898498","doi":"10.1088/0004-637x/738/1/25","title":"TeV AND MULTI-WAVELENGTH OBSERVATIONS OF Mrk 421 IN 2006-2008","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Science Foundation; Science Foundation Ireland; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution","keywords":"Physics; Blazar; Astrophysics; Observatory; Flux (metallurgy); Cherenkov radiation; Spectral line; Synchrotron; Astronomy; Active galactic nucleus; Telescope; Redshift; Cherenkov Telescope Array; Flare; Wavelength; Galaxy; Gamma ray; Detector; Nuclear physics; Optics","score_opus":0.03514049414222563,"score_gpt":0.22727181712672387,"score_spread":0.19213132298449825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968898498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99743915,0.00017498872,0.00021019943,0.000024587733,0.0000048214574,0.000007576527,0.0007502165,0.000043133314,0.0013452597],"genre_scores_gemma":[0.9921217,0.00017991335,0.0014516837,0.000046325138,0.000022195927,0.000009729928,0.0048637516,0.000030517247,0.001274295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997701,0.000016066906,0.000008547404,0.000070437716,0.0000874937,0.00004729664],"domain_scores_gemma":[0.9997172,0.000018639155,0.00010149287,0.000038349117,0.00005768849,0.000066594366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028144877,0.00029772762,0.00040031047,0.0007984038,0.0005512362,0.00047344167,0.00025420898,0.00034127958,0.0007703416],"category_scores_gemma":[0.00032117649,0.0002711334,0.00026146838,0.00068573805,0.00017545038,0.00028872534,0.00071515,0.00041578163,0.0003883955],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018978479,0.00038615518,0.7923705,0.0002575699,0.0002590205,0.0029061327,0.002659154,0.0028169057,0.14323744,0.0005012001,0.0031967433,0.049511366],"study_design_scores_gemma":[0.000014233114,0.00009763984,0.9946466,0.000008713698,0.000016177339,0.0004518874,0.00008542466,0.00042826848,0.0016559752,0.000027397811,0.0025594304,0.000008123918],"about_ca_topic_score_codex":0.004646197,"about_ca_topic_score_gemma":0.021922346,"teacher_disagreement_score":0.004646197,"about_ca_system_score_codex":0.00033483194,"about_ca_system_score_gemma":0.0002424163,"threshold_uncertainty_score":0.009238303},"labels":[],"label_agreement":null},{"id":"W1968961601","doi":"10.1086/340897","title":"The Distance to Clusters: Correcting for Asphericity","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cluster (spacecraft); Hydrostatic equilibrium; Measure (data warehouse); Line (geometry); Galaxy cluster; Gravitational lens; Distribution (mathematics); Gravitation; Weak gravitational lensing","score_opus":0.011246958533832051,"score_gpt":0.21810437141788727,"score_spread":0.2068574128840552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968961601","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.67730933,0.00090827164,0.31162563,0.00043589782,0.00026149116,0.000105427025,0.0022686617,0.0038669729,0.003218308],"genre_scores_gemma":[0.81536365,0.00023610432,0.1801683,0.00009410695,0.00004995519,0.000040513285,0.0015164263,0.00056694576,0.001963977],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99850625,0.00023739964,0.000093005336,0.0006742292,0.00038602948,0.0001030654],"domain_scores_gemma":[0.99387956,0.00093067845,0.0012276717,0.002422861,0.0013021776,0.00023697662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018269888,0.00095497456,0.0005069755,0.0018902898,0.0011114479,0.0008571906,0.0011445229,0.00066641107,0.0009197811],"category_scores_gemma":[0.014415068,0.0004907465,0.0005219623,0.0020084288,0.00054537953,0.00069250603,0.0011181346,0.0008834292,0.0007813869],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004123191,0.00007360353,0.52323955,0.00025075692,0.0010593226,0.000290783,0.0006732796,0.12331526,0.057606455,0.008828542,0.007374519,0.27687556],"study_design_scores_gemma":[0.000056798246,0.00011623863,0.64313,0.000029072851,0.00023492405,0.0006347954,0.000225273,0.25143728,0.07885852,0.007449194,0.017631749,0.00019613426],"about_ca_topic_score_codex":0.028801356,"about_ca_topic_score_gemma":0.03869445,"teacher_disagreement_score":0.028801356,"about_ca_system_score_codex":0.0009667694,"about_ca_system_score_gemma":0.0014109879,"threshold_uncertainty_score":0.057267427},"labels":[],"label_agreement":null},{"id":"W1968999134","doi":"10.1086/587022","title":"The Persistence of Universal Halo Profiles","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Substructure; Halo; Phase space; Instability; Cutoff; Astrophysics; Isotropy; Mass distribution; Distribution function; Classical mechanics; Galaxy; Mechanics; Quantum mechanics","score_opus":0.011703484118749982,"score_gpt":0.21944469153575769,"score_spread":0.2077412074170077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1968999134","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99495065,0.000026734915,0.0040637744,0.000028873199,0.0000023551183,0.0000061786095,0.000028220305,0.00009989132,0.0007933098],"genre_scores_gemma":[0.99945337,0.000009513099,0.00045044566,0.0000039248575,6.404019e-7,0.0000019830243,0.00001577468,0.0000075407834,0.00005678573],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998814,0.000028862452,0.000005674894,0.000020597028,0.000021800279,0.00004162949],"domain_scores_gemma":[0.9993149,0.00017165979,0.00014799085,0.00018412912,0.000066414104,0.00011486673],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037340957,0.00017514534,0.00020250966,0.00028887182,0.00031939292,0.00048824045,0.00040300968,0.00021541209,0.0008956203],"category_scores_gemma":[0.0028596285,0.0001767239,0.00030570547,0.00014576594,0.0007313957,0.0005425264,0.0007407431,0.000370625,0.00005672597],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006611047,0.00018272817,0.15314445,0.00026205348,0.00049119757,0.0017835499,0.0020989196,0.5775342,0.12870422,0.111906216,0.0010961934,0.022135124],"study_design_scores_gemma":[0.00007822277,0.00017292907,0.038349565,0.000022112596,0.000080229736,0.00031462943,0.00025633367,0.9183985,0.020580988,0.020413125,0.0012821611,0.000051125924],"about_ca_topic_score_codex":0.0028817689,"about_ca_topic_score_gemma":0.0016557524,"teacher_disagreement_score":0.0028817689,"about_ca_system_score_codex":0.000411561,"about_ca_system_score_gemma":0.00026458397,"threshold_uncertainty_score":0.0057299733},"labels":[],"label_agreement":null},{"id":"W1969181702","doi":"10.1086/423338","title":"A Central X-Ray Source in the Nonthermal Radio Nebula DA 495","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics; University of Manitoba","funders":"","keywords":"ROSAT; Physics; Astrophysics; Nebula; Supernova remnant; Crab Nebula; Emission nebula; Flux (metallurgy); Astronomy; Neutron star; Pulsar wind nebula; Supernova; Pulsar; Galaxy; Stars","score_opus":0.01047540047660772,"score_gpt":0.218697568444065,"score_spread":0.20822216796745727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969181702","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99661416,0.00036226233,0.0005350695,0.000032262295,0.0000143430925,0.000011739797,0.0002213376,0.00003668961,0.002172107],"genre_scores_gemma":[0.99865156,0.00005518812,0.0004729762,0.000024152157,0.000015480187,0.0000036955298,0.00032026038,0.0000022063123,0.0004545337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999523,0.0000030182634,0.0000027786011,0.000017989603,0.0000141440305,0.000009800171],"domain_scores_gemma":[0.9998677,0.000009169049,0.000056200992,0.000019322519,0.000009595162,0.000037932452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007532941,0.00021228817,0.00016296761,0.0003310772,0.0005028848,0.00046784108,0.00026648474,0.00023092047,0.0018042825],"category_scores_gemma":[0.00014886218,0.00008881366,0.000109397944,0.00025944875,0.00020880165,0.00018209658,0.0005742783,0.000120651704,0.00053566485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086913357,0.00025374017,0.4940582,0.00019533408,0.00010688562,0.012919722,0.0009845033,0.00034316775,0.44216505,0.0036343364,0.0020810494,0.04238892],"study_design_scores_gemma":[0.00005147462,0.0005559449,0.9531557,0.000033949396,0.00007473374,0.013741399,0.00024706003,0.0010933001,0.019684087,0.0006128721,0.010725726,0.000023735873],"about_ca_topic_score_codex":0.0013372157,"about_ca_topic_score_gemma":0.002782585,"teacher_disagreement_score":0.0018042825,"about_ca_system_score_codex":0.00014765095,"about_ca_system_score_gemma":0.00010193003,"threshold_uncertainty_score":0.0060359836},"labels":[],"label_agreement":null},{"id":"W1969233909","doi":"10.1088/0004-637x/785/2/121","title":"REVEALING THE NATURE OF THE ULX AND X-RAY POPULATION OF THE SPIRAL GALAXY NGC 4088","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Galaxy; Luminosity; Supermassive black hole; Black hole (networking); Population; Spiral galaxy; Eddington luminosity; ROSAT","score_opus":0.0067505179040111786,"score_gpt":0.21835741047268342,"score_spread":0.21160689256867224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969233909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994466,0.00004247169,0.000032499236,0.0000068467953,2.6324483e-7,9.651657e-7,0.00004328455,0.0000049058463,0.00042221972],"genre_scores_gemma":[0.9994062,0.00004937002,0.00014403914,0.00000509601,0.0000014796499,0.000002322377,0.00017193305,0.000002119248,0.00021760608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999291,0.0000060541815,0.000003796328,0.000019743093,0.000014817299,0.00002649002],"domain_scores_gemma":[0.99979264,0.000016684118,0.00009080929,0.000023625758,0.000020965223,0.000055321198],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000095212956,0.00017415517,0.00011509306,0.00095249026,0.00019771479,0.00030890448,0.00020372997,0.0001656163,0.00089002954],"category_scores_gemma":[0.00030579144,0.00013118582,0.00010083268,0.00041408374,0.00020975586,0.00020224298,0.00043632815,0.00010323336,0.00025513582],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018623726,0.00003762869,0.90810174,0.000028334256,0.000030292646,0.00037754426,0.0007565028,0.0005568863,0.074849434,0.000450361,0.00021992884,0.014405148],"study_design_scores_gemma":[0.0000032528826,0.000038176335,0.9978644,0.000004341044,0.0000048473125,0.00029930548,0.0001192266,0.0003693172,0.00062055606,0.00006324792,0.00061015907,0.0000032362047],"about_ca_topic_score_codex":0.004886933,"about_ca_topic_score_gemma":0.006723088,"teacher_disagreement_score":0.004886933,"about_ca_system_score_codex":0.00027791035,"about_ca_system_score_gemma":0.0001065803,"threshold_uncertainty_score":0.009716988},"labels":[],"label_agreement":null},{"id":"W1969260612","doi":"10.1086/322266","title":"The Interstellar Medium of M32","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Elliptical galaxy; Astronomy; Galaxy; Spiral galaxy; Local Group; Barred spiral galaxy; Irregular galaxy; Lenticular galaxy; Interstellar medium; Interacting galaxy; Dwarf galaxy","score_opus":0.009653756849208734,"score_gpt":0.23594089335133514,"score_spread":0.2262871365021264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969260612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98192924,0.0023102418,0.00030099656,0.00011986273,0.000026195275,0.0000076697115,0.00013892539,0.000013842553,0.015152959],"genre_scores_gemma":[0.9974657,0.00059062184,0.00019335303,0.000040565075,0.00001460606,0.000004115116,0.00020530354,0.0000028027512,0.0014828484],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993885,0.0000065112526,0.0000019247814,0.000015285585,0.000013816989,0.00002358286],"domain_scores_gemma":[0.99989426,0.000014541373,0.000024732431,0.000011382002,0.000013452484,0.000041680432],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009045593,0.00021065677,0.00013681373,0.00031903747,0.00053439784,0.00085815537,0.0001798338,0.0002896335,0.0028514995],"category_scores_gemma":[0.00039041197,0.000104666375,0.000074214324,0.00022089302,0.00028215616,0.0007005759,0.0010724646,0.00029170583,0.00088066753],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010404467,0.00012286466,0.11756047,0.0003221325,0.000057444213,0.0037511918,0.0023934017,0.00045405008,0.82626486,0.013298071,0.0018820295,0.032853007],"study_design_scores_gemma":[0.00014649902,0.0021657378,0.70913756,0.00019216131,0.00010371883,0.012574744,0.00793134,0.00215101,0.11034403,0.011447261,0.14369103,0.000114846465],"about_ca_topic_score_codex":0.0017792823,"about_ca_topic_score_gemma":0.0016992262,"teacher_disagreement_score":0.0028514995,"about_ca_system_score_codex":0.00025947817,"about_ca_system_score_gemma":0.0001842506,"threshold_uncertainty_score":0.009539187},"labels":[],"label_agreement":null},{"id":"W1969309507","doi":"10.1086/422384","title":"Measurement of the Abundance of Radioactive<sup>10</sup>Be and Other Light Isotopes in Cosmic Radiation up to 2 GeV Nucleon<sup>−1</sup>with the Balloon‐borne Instrument ISOMAX","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Nuclear physics; Cosmic ray; Nucleon; Isotopes of beryllium; Rigidity (electromagnetism); Isotope; Beryllium; Muon","score_opus":0.013311335507470481,"score_gpt":0.2368765488885444,"score_spread":0.2235652133810739,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969309507","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99082446,0.00026300855,0.0042818203,0.000040497787,0.000010067822,0.000017274324,0.0006561689,0.000091428774,0.0038153497],"genre_scores_gemma":[0.98772776,0.00029614073,0.0076650316,0.00005204869,0.000012089958,0.000035107143,0.0015034871,0.00006144221,0.0026468516],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9997745,0.00003521312,0.000008809335,0.00006395383,0.00008650527,0.000030925166],"domain_scores_gemma":[0.999696,0.000051680556,0.00009302668,0.000035437206,0.00009244864,0.000031299125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034553144,0.00030807185,0.00017894963,0.00060568075,0.00031747762,0.000326673,0.00052048627,0.0002563193,0.0009008358],"category_scores_gemma":[0.0005351933,0.00028684232,0.00013886846,0.00047376964,0.00025357865,0.00026640345,0.0003223406,0.0003243137,0.0002237707],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011583554,0.00004530035,0.12089513,0.00007903513,0.000078367215,0.00016381411,0.00019629442,0.0006130596,0.86564714,0.000830592,0.00035355514,0.009939458],"study_design_scores_gemma":[0.000059849826,0.0004952207,0.47082144,0.000021376309,0.00010791344,0.0005888613,0.00011389499,0.0040027546,0.5127212,0.00025000997,0.010779413,0.000038016027],"about_ca_topic_score_codex":0.003142552,"about_ca_topic_score_gemma":0.008484445,"teacher_disagreement_score":0.003142552,"about_ca_system_score_codex":0.0005936725,"about_ca_system_score_gemma":0.00030458136,"threshold_uncertainty_score":0.0062485337},"labels":[],"label_agreement":null},{"id":"W1969322924","doi":"10.1088/0004-637x/731/2/86","title":"DISCOVERY AND COSMOLOGICAL IMPLICATIONS OF SPT-CL J2106-5844, THE MOST MASSIVE KNOWN CLUSTER AT z&gt;1","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; McGill University; W. M. Keck Foundation; Deutsche Forschungsgemeinschaft; Massachusetts Institute of Technology; Canada Research Chairs; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Galaxy cluster; Galaxy; Brightest cluster galaxy; Redshift; Interacting galaxy; Cosmology; Cluster (spacecraft); Luminosity; Galaxy formation and evolution","score_opus":0.012915725758511427,"score_gpt":0.21382693229868846,"score_spread":0.20091120654017702,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969322924","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988894,0.000040116178,0.000050258976,0.000114560455,0.0000050419535,0.000003332127,0.00008241987,0.000007640893,0.00080738607],"genre_scores_gemma":[0.9993538,0.000028784485,0.00014048099,0.000035099285,0.000014726962,0.0000019356169,0.00016389499,0.0000021332314,0.00025914513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994123,0.000004750884,0.0000017828645,0.000017466136,0.00001505935,0.000019722556],"domain_scores_gemma":[0.99976724,0.000010423466,0.000062253144,0.000012373262,0.000021512635,0.00012618006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013760777,0.00014131282,0.0001821789,0.00078352727,0.0012556094,0.0005974709,0.00025478963,0.00026712348,0.002525159],"category_scores_gemma":[0.00035275074,0.00014381281,0.00009320618,0.0004753196,0.0004565184,0.0002950803,0.00077211135,0.00035444496,0.0003054223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023088662,0.00009809668,0.9564845,0.000020261996,0.000033855074,0.0030541383,0.0007183782,0.0001391395,0.026238319,0.0011666658,0.0016810861,0.010134718],"study_design_scores_gemma":[0.00001083859,0.000069397116,0.9947802,0.0000038396374,0.0000105774825,0.0014912041,0.0003412713,0.00035417275,0.000525428,0.0002567746,0.0021509083,0.000005383908],"about_ca_topic_score_codex":0.0054215775,"about_ca_topic_score_gemma":0.008761048,"teacher_disagreement_score":0.0054215775,"about_ca_system_score_codex":0.0003545636,"about_ca_system_score_gemma":0.00015810571,"threshold_uncertainty_score":0.010780036},"labels":[],"label_agreement":null},{"id":"W1969426120","doi":"10.1086/422337","title":"Magnetars: Time Evolution, Superfluid Properties, and the Mechanism of Magnetic Field Decay","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Superfluidity; Magnetic field; Neutron star; Thermal conduction; Condensation; Field (mathematics); Thermal","score_opus":0.008104312926445091,"score_gpt":0.23509586531962037,"score_spread":0.22699155239317528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969426120","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9886884,0.00020561472,0.008343805,0.000108483684,0.000011669135,0.000011610968,0.000114758,0.000110319284,0.0024053622],"genre_scores_gemma":[0.99791414,0.000091263006,0.001151461,0.000012001943,0.000004513929,0.000009698691,0.00008522913,0.000030974723,0.00070063956],"study_design_codex":"simulation_or_modeling","study_design_gemma":"not_applicable","domain_scores_codex":[0.99994814,0.000014286614,0.000002202227,0.000008200881,0.0000090627655,0.000018166675],"domain_scores_gemma":[0.9997272,0.0000774405,0.00009887538,0.00002877679,0.00003325789,0.00003442315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003794963,0.00028028525,0.00029049357,0.00036773237,0.0003388825,0.00051481085,0.000605875,0.0006388906,0.0012476234],"category_scores_gemma":[0.0012924506,0.00023610453,0.00037677938,0.0003287726,0.0005787966,0.0007943254,0.00031570406,0.0003364031,0.00016819379],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023757879,0.00005931154,0.027373305,0.00007875178,0.000069120644,0.00036648504,0.00012926965,0.9171123,0.0137542095,0.036085326,0.00046241292,0.004271886],"study_design_scores_gemma":[0.000054457043,0.00005712271,0.00685487,0.000005528975,0.00002104038,0.0000741309,0.000032698837,0.9864633,0.002423644,0.003570844,0.00042954786,0.000012708985],"about_ca_topic_score_codex":0.004922181,"about_ca_topic_score_gemma":0.0026650892,"teacher_disagreement_score":0.004922181,"about_ca_system_score_codex":0.0006120256,"about_ca_system_score_gemma":0.00028015327,"threshold_uncertainty_score":0.009787083},"labels":[],"label_agreement":null},{"id":"W1969434326","doi":"10.1086/429219","title":"Discovery of Spectroscopic Variations in the DAB White Dwarf GD 323","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Helium; Hydrogen; Amplitude; Atmosphere (unit); Absorption spectroscopy; Spectral line; Absorption (acoustics)","score_opus":0.009150262026128867,"score_gpt":0.23238625185565928,"score_spread":0.2232359898295304,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969434326","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99929047,0.000059418668,0.00015001725,0.000015052117,0.00000257835,0.0000030198753,0.000100541765,0.000009374246,0.00036947816],"genre_scores_gemma":[0.999569,0.00002690639,0.00016327498,0.000011405166,0.0000020516939,0.0000017460076,0.00012469279,0.000002078999,0.00009882702],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995697,0.0000025310403,0.000002711368,0.000015805808,0.00001243551,0.000009580713],"domain_scores_gemma":[0.9999031,0.0000056104523,0.00003709342,0.000011821437,0.000014751986,0.000027674936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006984179,0.0001503092,0.00015330197,0.0003323862,0.0003385076,0.0002970542,0.00016015243,0.00019129811,0.00022722008],"category_scores_gemma":[0.0002543433,0.00009204557,0.00011831724,0.00024335743,0.00021789318,0.00009578631,0.00034688914,0.00018825853,0.00012247787],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018467483,0.000029394065,0.6679703,0.00004057665,0.000036394467,0.00089336274,0.0007851001,0.0001861877,0.31742632,0.00039070836,0.0002846962,0.011772291],"study_design_scores_gemma":[0.000007471904,0.000111831876,0.98588866,0.0000054495154,0.000023346418,0.001222982,0.00026668384,0.00034037844,0.008434034,0.00022645126,0.003464676,0.00000803079],"about_ca_topic_score_codex":0.0053498438,"about_ca_topic_score_gemma":0.009384346,"teacher_disagreement_score":0.0053498438,"about_ca_system_score_codex":0.0003410953,"about_ca_system_score_gemma":0.000116137526,"threshold_uncertainty_score":0.010637403},"labels":[],"label_agreement":null},{"id":"W1969452322","doi":"10.1086/324752","title":"Multiwavelength Studies of PSR J1420−6048, a Young Pulsar in the Kookaburra","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Nebula; Polarization (electrochemistry); Infrared; Millisecond pulsar; Radio spectrum; Pulsar wind nebula; Radio astronomy; High resolution","score_opus":0.0335269908695091,"score_gpt":0.28985313100899945,"score_spread":0.25632614013949034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969452322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99941826,0.00009771487,0.00005742044,0.0000062074955,0.000001369435,0.0000020584494,0.00003404668,0.0000043627356,0.00037861257],"genre_scores_gemma":[0.9987374,0.00019226357,0.00040882593,0.00001734036,0.0000122087895,0.000006416289,0.0002541522,0.00000593921,0.00036547516],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995196,0.0000023010177,0.000003051401,0.000014807665,0.000012270906,0.00001557926],"domain_scores_gemma":[0.99972194,0.000019598789,0.00014649663,0.000018016806,0.000025640964,0.00006834982],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007689961,0.00021802368,0.00020627512,0.0009918257,0.00040741172,0.0003197567,0.00021054914,0.00025264977,0.0006247995],"category_scores_gemma":[0.00023746202,0.00018668675,0.00012824655,0.0005576337,0.00022389338,0.000303785,0.0004783251,0.00020262324,0.0003043332],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040733657,0.00015941751,0.47992873,0.00009258126,0.00006540922,0.002815948,0.001173713,0.00026633628,0.49873126,0.00023670499,0.00021629583,0.01590633],"study_design_scores_gemma":[0.0000072870475,0.00014641146,0.993131,0.000005978143,0.00001697184,0.0015970307,0.00022682163,0.0001380831,0.0037565606,0.00005458634,0.0009140019,0.000005304763],"about_ca_topic_score_codex":0.00097148726,"about_ca_topic_score_gemma":0.0026975384,"teacher_disagreement_score":0.0009918257,"about_ca_system_score_codex":0.00012966854,"about_ca_system_score_gemma":0.000064262036,"threshold_uncertainty_score":0.002090156},"labels":[],"label_agreement":null},{"id":"W1969581871","doi":"10.1086/514330","title":"Where the Blue Stragglers Roam: Searching for a Link between Formation and Environment","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Blue straggler; Globular cluster; Population; Cluster (spacecraft); Astrophysics; Physics; Stars; Computer science; Demography","score_opus":0.016158111538996295,"score_gpt":0.23949699680790956,"score_spread":0.22333888526891327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969581871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994748,0.000051811778,0.0001612725,0.000011084524,4.8141493e-7,0.0000017525373,0.000023586015,0.000005663997,0.00026946084],"genre_scores_gemma":[0.99950695,0.0000372599,0.00023923564,0.000008651869,0.0000011044871,0.0000016736049,0.00004784106,0.0000045847746,0.0001528052],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979883,0.00006491813,0.0000069358753,0.00004666558,0.000030305495,0.000052411408],"domain_scores_gemma":[0.99884987,0.00022460191,0.00042617726,0.00014532664,0.00013596045,0.00021807729],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004042718,0.00012914732,0.00023217159,0.0009703749,0.00042675206,0.000692548,0.00030350883,0.00021693276,0.0009682083],"category_scores_gemma":[0.0018985277,0.00014658272,0.0001081706,0.00062415964,0.00042317237,0.0005471076,0.0006406252,0.00017180401,0.00030939758],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000099538,0.0000172497,0.990871,0.000008319222,0.00002499014,0.0000734955,0.00051796535,0.00016386724,0.0027874517,0.00020702771,0.000110200905,0.005118774],"study_design_scores_gemma":[0.0000029253981,0.00006548521,0.9967854,0.0000056702643,0.000013446888,0.0001637006,0.0006764439,0.00066923356,0.00081087113,0.0002668235,0.0005337873,0.000006189094],"about_ca_topic_score_codex":0.004819552,"about_ca_topic_score_gemma":0.010012205,"teacher_disagreement_score":0.004819552,"about_ca_system_score_codex":0.00023984048,"about_ca_system_score_gemma":0.00021195647,"threshold_uncertainty_score":0.009582996},"labels":[],"label_agreement":null},{"id":"W1969594725","doi":"10.1088/0004-637x/743/1/51","title":"FAST MAGNETIC RECONNECTION AND SPONTANEOUS STOCHASTICITY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":179,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gyroradius; Physics; Magnetic reconnection; Magnetohydrodynamics; Magnetic field; Turbulence; Magnetic flux; Magnetic energy; Classical mechanics; Computational physics; Mechanics; Quantum electrodynamics; Magnetization; Quantum mechanics","score_opus":0.009276373165822723,"score_gpt":0.19327444869839408,"score_spread":0.18399807553257136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969594725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9075701,0.0013427701,0.07382815,0.00066189875,0.00006569855,0.000017788812,0.00006173403,0.0002953869,0.016156457],"genre_scores_gemma":[0.99786276,0.0002126945,0.0012758287,0.00002442326,0.000029878578,0.0000055717587,0.000021430205,0.000009026012,0.00055840897],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997274,0.000064773056,0.000013066654,0.000054859163,0.00009218161,0.00004765165],"domain_scores_gemma":[0.998548,0.0006671364,0.0004161374,0.00019118957,0.00009928703,0.00007824964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034815772,0.00018370994,0.00012475063,0.00025848308,0.00027797185,0.00080517505,0.00035363523,0.00029119814,0.00079078175],"category_scores_gemma":[0.0026070226,0.0001251857,0.00020978547,0.00015735326,0.001238733,0.0010384629,0.0007844096,0.0003799646,0.00012482714],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000091906826,0.00007571082,0.03266833,0.00012456762,0.000038499154,0.000602701,0.0005108909,0.18084143,0.018364822,0.74157435,0.0014496967,0.023657095],"study_design_scores_gemma":[0.00003293651,0.00013934291,0.025623063,0.00002481081,0.000021610904,0.00081536145,0.00021539639,0.47574285,0.0084913075,0.48428878,0.0045602093,0.00004433483],"about_ca_topic_score_codex":0.00083079515,"about_ca_topic_score_gemma":0.00042848813,"teacher_disagreement_score":0.00083079515,"about_ca_system_score_codex":0.0003971637,"about_ca_system_score_gemma":0.00032459892,"threshold_uncertainty_score":0.0028815866},"labels":[],"label_agreement":null},{"id":"W1969655752","doi":"10.1088/0004-637x/791/1/28","title":"CARBON-RICH DUST PAST THE ASYMPTOTIC GIANT BRANCH: ALIPHATICS, AROMATICS, AND FULLERENES IN THE MAGELLANIC CLOUDS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Western University","funders":"Science and Technology Facilities Council","keywords":"Spectral line; Fullerene; Line-of-sight; Infrared; Line (geometry); Feature (linguistics); Emission spectrum; Cosmic dust","score_opus":0.009331772008918424,"score_gpt":0.21794159414148684,"score_spread":0.2086098221325684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969655752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99944574,0.000089986774,0.000058569924,0.000008786791,9.1174195e-7,0.0000010971978,0.000027844506,0.000004835693,0.00036215544],"genre_scores_gemma":[0.99968743,0.00003187906,0.000089309106,0.000007885903,0.0000031533432,6.601841e-7,0.00009393154,0.0000021884186,0.000083486135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999237,0.000003310633,0.0000040645323,0.000021896178,0.000023946086,0.000023030569],"domain_scores_gemma":[0.9998272,0.000016164715,0.00004753385,0.000013428319,0.000036631438,0.00005902705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000107414584,0.00019146946,0.0001906184,0.0010343958,0.0005433218,0.0003930913,0.0002851322,0.00031319755,0.00049044396],"category_scores_gemma":[0.00021769092,0.00011924784,0.00016758418,0.0007128304,0.0003466739,0.00031861255,0.00035949802,0.0002149236,0.000127747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027652833,0.000062382176,0.66367,0.000046360707,0.00005091883,0.0008434583,0.0004661414,0.0004131214,0.32203946,0.00023611772,0.00012964492,0.011765923],"study_design_scores_gemma":[0.0000028748223,0.000023306133,0.9962913,0.000002501009,0.0000070811893,0.00019682816,0.000088046894,0.00020784975,0.002925393,0.000052861324,0.0001999844,0.0000020298746],"about_ca_topic_score_codex":0.0043336456,"about_ca_topic_score_gemma":0.005697611,"teacher_disagreement_score":0.0043336456,"about_ca_system_score_codex":0.00050444074,"about_ca_system_score_gemma":0.0001061954,"threshold_uncertainty_score":0.008616865},"labels":[],"label_agreement":null},{"id":"W1969779249","doi":"10.1086/508656","title":"On the Formation of Extended Galactic Disks by Tidally Disrupted Dwarf Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Dwarf galaxy; Milky Way; Galaxy; Stellar dynamics; Spiral galaxy; Galactic halo; Circular orbit; Thick disk; Satellite galaxy; Disc","score_opus":0.006186427770450402,"score_gpt":0.20940942222465567,"score_spread":0.20322299445420527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969779249","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984596,0.00006133434,0.0004320679,0.000049164995,0.0000035500589,0.000004674972,0.0000391021,0.000016744529,0.00093378435],"genre_scores_gemma":[0.99933237,0.000070114125,0.00028949525,0.000021841883,0.0000038218545,0.000004329915,0.000050199855,0.0000087321505,0.00021911075],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999056,0.000029533141,0.0000039101606,0.000014395278,0.000011099819,0.000035463774],"domain_scores_gemma":[0.99942124,0.00022483972,0.00010135741,0.00006145252,0.000043893513,0.00014725169],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043267087,0.00039570057,0.0005550989,0.0004435481,0.00082295673,0.0010083882,0.0007897301,0.0006851083,0.0013240518],"category_scores_gemma":[0.0018205808,0.000370827,0.00047020052,0.00036408246,0.0013319084,0.0010652158,0.0010141477,0.00036161212,0.00019682605],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043990987,0.00013374769,0.07510006,0.00006809803,0.00017536429,0.00092538446,0.0005462385,0.9066755,0.005533433,0.0066359034,0.0004586117,0.003307701],"study_design_scores_gemma":[0.00031687037,0.00027488882,0.03401721,0.000022150703,0.00008082225,0.00015726514,0.0004665944,0.9562688,0.0011665095,0.006161761,0.001025679,0.000041414034],"about_ca_topic_score_codex":0.017010694,"about_ca_topic_score_gemma":0.013639922,"teacher_disagreement_score":0.017010694,"about_ca_system_score_codex":0.00095059274,"about_ca_system_score_gemma":0.00048129703,"threshold_uncertainty_score":0.03382337},"labels":[],"label_agreement":null},{"id":"W1969814907","doi":"10.1086/504833","title":"Structure of Passive Circumstellar Disks: Beyond the Two‐Temperature Approximation","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Research Canada; University of Toronto","funders":"","keywords":"Physics; Wavelength; Computational physics; Radiation; Moment (physics); Point (geometry); Optics; Simple (philosophy); Heavy traffic approximation; Astrophysics; Classical mechanics; Geometry; Mathematics","score_opus":0.003744400875806272,"score_gpt":0.2101795704220823,"score_spread":0.20643516954627603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969814907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9279757,0.0006708454,0.0645559,0.0001581544,0.00001544185,0.000026540634,0.00014279943,0.00016891754,0.00628565],"genre_scores_gemma":[0.99618214,0.00013348376,0.0029349055,0.000014172953,0.000011604698,0.000008599832,0.00007167276,0.00002365968,0.0006197179],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999534,0.000009080081,0.000002210552,0.00001262844,0.000014338722,0.000008338075],"domain_scores_gemma":[0.9998264,0.000035752517,0.00004038696,0.0000382796,0.00003232615,0.000026896741],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109265864,0.00027690825,0.00020726658,0.00028990314,0.00024840387,0.0009894487,0.0008675837,0.00053352164,0.0005701559],"category_scores_gemma":[0.00072953914,0.0002226487,0.00020423351,0.00020938479,0.00046540418,0.00084656454,0.00045039863,0.0002569327,0.00023110815],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032064156,0.0002925386,0.05042226,0.00027954852,0.00009739264,0.001906609,0.0010476804,0.5577365,0.23085497,0.119656555,0.0015108966,0.035874356],"study_design_scores_gemma":[0.00005432533,0.00007751421,0.02406638,0.000012255502,0.000013387909,0.00045339874,0.00006977553,0.93542993,0.006849343,0.031447254,0.0015061422,0.000020255879],"about_ca_topic_score_codex":0.0009393225,"about_ca_topic_score_gemma":0.0003743944,"teacher_disagreement_score":0.0009894487,"about_ca_system_score_codex":0.0003417173,"about_ca_system_score_gemma":0.0001535375,"threshold_uncertainty_score":0.0024793148},"labels":[],"label_agreement":null},{"id":"W1969831933","doi":"10.1088/0004-637x/746/1/33","title":"OBSERVATION OF ANISOTROPY IN THE GALACTIC COSMIC-RAY ARRIVAL DIRECTIONS AT 400 TeV WITH ICECUBE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":157,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Marsden Fund; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Vetenskapsrådet; Knut och Alice Wallenbergs Stiftelse; Fonds Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; Belgian Federal Science Policy Office; Bundesministerium für Bildung und Forschung; Office of Polar Programs; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; University of Wisconsin-Madison; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Cosmic ray; Sky; Anisotropy; Muon; Astrophysics; Angular resolution (graph drawing); Astronomy; Observatory; COSMIC cancer database; Ultra-high-energy cosmic ray; Nuclear physics","score_opus":0.014213188739523758,"score_gpt":0.22826486789770284,"score_spread":0.21405167915817908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969831933","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9883541,0.00015928186,0.0014833306,0.000054743796,0.000012714294,0.0000151304685,0.002232813,0.00012109242,0.0075667137],"genre_scores_gemma":[0.9889338,0.00019801102,0.003683449,0.000046771776,0.000027828788,0.00002036951,0.0061591347,0.000063853644,0.00086684607],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977285,0.000032455635,0.000009925614,0.000046166173,0.000087906854,0.00005067553],"domain_scores_gemma":[0.9992969,0.00014716655,0.00022147522,0.00013458297,0.00013247902,0.00006746533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037120847,0.0002259071,0.00028745036,0.0006656182,0.00026775405,0.00053276453,0.00017889333,0.00016546951,0.0008856117],"category_scores_gemma":[0.0007753485,0.00017439146,0.00016182763,0.0011674094,0.00021872869,0.00031200395,0.0005122396,0.00034580776,0.0002576237],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018398198,0.00016359195,0.78362,0.0001040699,0.00028874358,0.0010450208,0.0006924835,0.00534768,0.16176139,0.0013179646,0.003695467,0.04012374],"study_design_scores_gemma":[0.00002007696,0.00009815379,0.9724157,0.000018848797,0.000043326298,0.0004841963,0.0000976348,0.0026171086,0.016793583,0.00024033179,0.007152038,0.000018975627],"about_ca_topic_score_codex":0.0036225063,"about_ca_topic_score_gemma":0.009589346,"teacher_disagreement_score":0.0036225063,"about_ca_system_score_codex":0.00037984288,"about_ca_system_score_gemma":0.00025885648,"threshold_uncertainty_score":0.007202804},"labels":[],"label_agreement":null},{"id":"W1969881699","doi":"10.1086/322298","title":"Evolution of Solar Filament Channels Observed during a Major Poleward Surge of Photospheric Magnetic Flux","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Protein filament; Sunspot; Flux (metallurgy); Magnetic flux; Astrophysics; Photosphere; Solar observatory; Polar; Equator; Polarity (international relations); Geophysics; Astronomy; Latitude; Magnetic field","score_opus":0.008385085670349821,"score_gpt":0.19919686093272732,"score_spread":0.1908117752623775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969881699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959831,0.00013167175,0.00046048602,0.000024622512,0.0000070151136,0.0000101858095,0.0004610058,0.00006441708,0.0028575],"genre_scores_gemma":[0.99850357,0.000049553113,0.0005035973,0.000011307465,0.000007933566,0.000008480287,0.00050314196,0.000020084932,0.00039229693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994075,0.000002950494,0.0000017866935,0.000017173856,0.000013477522,0.000023817038],"domain_scores_gemma":[0.9997743,0.000026691792,0.000058054557,0.0000141351475,0.00004114636,0.00008575138],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000080356745,0.00011059209,0.00015570891,0.0006745578,0.00043158626,0.0005593451,0.00018446593,0.00035169232,0.001251089],"category_scores_gemma":[0.00026855373,0.00012433273,0.0001853222,0.00034687095,0.00019937295,0.00025715766,0.00041776252,0.0003018631,0.00021275543],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054493704,0.00012904232,0.7059698,0.00008421066,0.00010132918,0.002315694,0.0014267279,0.0020677166,0.2616233,0.0015073137,0.001574729,0.022655156],"study_design_scores_gemma":[0.000005955889,0.000048395388,0.98984736,0.000012135237,0.000018358047,0.00035703773,0.00028481305,0.0018755099,0.004516812,0.00016886528,0.0028514669,0.000013268596],"about_ca_topic_score_codex":0.0025920235,"about_ca_topic_score_gemma":0.0036892812,"teacher_disagreement_score":0.0025920235,"about_ca_system_score_codex":0.00036888456,"about_ca_system_score_gemma":0.0001536428,"threshold_uncertainty_score":0.0051538944},"labels":[],"label_agreement":null},{"id":"W1969896933","doi":"10.1088/0004-637x/756/2/136","title":"HYDROGEN FLUORIDE IN HIGH-MASS STAR-FORMING REGIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"Agence Nationale de la Recherche","keywords":"Astrophysics; Hydrogen; Absorption (acoustics); Interstellar cloud; Outflow; Desorption; Star formation; Astrochemistry; Physics; Abundance (ecology); Interstellar medium; Chemistry; Molecular cloud; Astronomy; Stars; Galaxy; Optics","score_opus":0.012842077393507689,"score_gpt":0.23765326813018128,"score_spread":0.2248111907366736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1969896933","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992835,0.00024977376,0.000107517066,0.0000081257385,5.4248744e-7,0.0000011302582,0.00003800281,0.0000052092137,0.00030614863],"genre_scores_gemma":[0.99969673,0.00006193172,0.00013357695,0.0000037200907,0.0000017030809,7.083253e-7,0.000062472776,9.575091e-7,0.00003825997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994695,0.0000052913524,0.0000028226816,0.000018852843,0.000008932246,0.000017076314],"domain_scores_gemma":[0.9998361,0.000022058359,0.00008017107,0.000010111851,0.000017527786,0.00003401871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011499521,0.000120840305,0.00015714021,0.0005471504,0.00032997492,0.0003250479,0.00024110034,0.0002509467,0.0005025762],"category_scores_gemma":[0.00024306733,0.00010205315,0.00008434729,0.00034540085,0.00022214615,0.00019826,0.0002388772,0.00010375088,0.00009052436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018127296,0.000038543818,0.8314921,0.000053804833,0.000047737547,0.00035978033,0.0002845038,0.0010708234,0.1557989,0.00043353607,0.00013307139,0.010105962],"study_design_scores_gemma":[0.0000072339244,0.000040456438,0.9933183,0.000003888693,0.000012612302,0.00024616366,0.00008206524,0.00084081537,0.0048643616,0.00022293947,0.00035780604,0.0000033655056],"about_ca_topic_score_codex":0.008779583,"about_ca_topic_score_gemma":0.0068615098,"teacher_disagreement_score":0.008779583,"about_ca_system_score_codex":0.00041840662,"about_ca_system_score_gemma":0.000089225796,"threshold_uncertainty_score":0.017456949},"labels":[],"label_agreement":null},{"id":"W1970012634","doi":"10.1086/345345","title":"Wind Accretion and State Transitions in Cygnus X‐1","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Accretion (finance); Flux (metallurgy); Supergiant; Emission spectrum; Light curve; Ionization; Accretion disc; Spectral line","score_opus":0.010484689718568616,"score_gpt":0.2230101233216653,"score_spread":0.2125254336030967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970012634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99961,0.000031907886,0.00003138484,0.000011603413,0.0000012610271,0.0000044007415,0.00007345497,0.000004946674,0.00023094297],"genre_scores_gemma":[0.9992976,0.000030460666,0.00007195116,0.000010703891,0.0000028452325,0.000006609978,0.00031321266,0.000001967282,0.00026455437],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999936,0.000009516694,0.0000043772266,0.00001725074,0.000013391131,0.000019455887],"domain_scores_gemma":[0.9996093,0.000041667958,0.00023005868,0.000016630054,0.00004566978,0.000056740235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016602881,0.00018401393,0.00017941109,0.0005529834,0.00039670357,0.0005127618,0.00013453774,0.00029701003,0.0006753268],"category_scores_gemma":[0.0007425188,0.0001082197,0.00009620015,0.0003665431,0.00026230357,0.0001605893,0.00032864723,0.0002519255,0.00013159275],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007734826,0.00025635865,0.95593655,0.000027910455,0.000055949007,0.00066393585,0.0005512546,0.0009706046,0.028638981,0.00021926805,0.00023791926,0.011667895],"study_design_scores_gemma":[0.000010756934,0.00011457168,0.9967443,0.0000036458684,0.000008113705,0.00021885197,0.000074865144,0.0007561137,0.0016455636,0.00009350436,0.00032478714,0.000004990831],"about_ca_topic_score_codex":0.007886584,"about_ca_topic_score_gemma":0.01101221,"teacher_disagreement_score":0.007886584,"about_ca_system_score_codex":0.00040309227,"about_ca_system_score_gemma":0.00017953826,"threshold_uncertainty_score":0.015681386},"labels":[],"label_agreement":null},{"id":"W1970131072","doi":"10.1088/0004-637x/698/1/222","title":"THE SIGNATURE OF GALACTIC TIDES IN LOCAL GROUP DWARF SPHEROIDALS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Orbit (dynamics); Milky Way; RADIUS; Local Group; Stars; Halo; Galactic Center; Accretion (finance)","score_opus":0.007154416071616339,"score_gpt":0.25702475845294237,"score_spread":0.24987034238132602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970131072","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99266,0.000050877374,0.0007831772,0.0001378566,0.000019030642,0.00000934973,0.00048205277,0.00011548223,0.005742119],"genre_scores_gemma":[0.99852115,0.00002606194,0.0006102742,0.000027822223,0.000003976213,0.000005769026,0.00028755827,0.00002996057,0.00048749495],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99995303,0.000010979259,0.0000021813705,0.000010693357,0.000008039687,0.000015156724],"domain_scores_gemma":[0.99972695,0.00009301342,0.000033890366,0.000028234432,0.000030812655,0.00008711925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016289817,0.0002212598,0.00025644494,0.00027589028,0.00046998612,0.0005570949,0.00044591245,0.00047872143,0.0044639744],"category_scores_gemma":[0.00081843993,0.00015419435,0.00036988588,0.00024588118,0.00041316048,0.000267299,0.00038926178,0.0003934045,0.00024407032],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029711655,0.0001797544,0.092965335,0.00006438139,0.00011637182,0.00054374075,0.00033397364,0.8837042,0.007484027,0.005802634,0.003664581,0.0048438525],"study_design_scores_gemma":[0.00009790166,0.00010361572,0.035992082,0.000014527199,0.000023485174,0.00005071675,0.00020803865,0.959615,0.0007495054,0.0019474807,0.0011802838,0.000017363102],"about_ca_topic_score_codex":0.034977593,"about_ca_topic_score_gemma":0.026464049,"teacher_disagreement_score":0.034977593,"about_ca_system_score_codex":0.000580366,"about_ca_system_score_gemma":0.00040725368,"threshold_uncertainty_score":0.06954801},"labels":[],"label_agreement":null},{"id":"W1970196846","doi":"10.1088/0004-637x/709/2/644","title":"GALAXY STELLAR MASS ASSEMBLY BETWEEN 0.2 &lt;<i>z</i>&lt; 2 FROM THE S-COSMOS SURVEY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":697,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Stellar mass; Elliptical galaxy; Astronomy; Luminous infrared galaxy; Galaxy; Star formation; Galaxy formation and evolution","score_opus":0.01203541308204572,"score_gpt":0.2218783404252736,"score_spread":0.20984292734322788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970196846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9793027,0.00022013785,0.00052204286,0.000073468465,0.000011738686,0.000021759692,0.011783491,0.0001994189,0.007865087],"genre_scores_gemma":[0.9662652,0.00016181245,0.0012723639,0.000059334998,0.00002034547,0.000028350734,0.028353604,0.00005332651,0.0037856551],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999075,0.0000071531435,0.0000048717807,0.0000280384,0.000019172074,0.00003320016],"domain_scores_gemma":[0.9996007,0.000024006386,0.00012385561,0.000037537102,0.00011581865,0.00009816642],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022461223,0.00022783359,0.00017508656,0.0016433375,0.00018931263,0.00046033552,0.00018581975,0.00017141293,0.0025690822],"category_scores_gemma":[0.00041565602,0.00010330269,0.0002789494,0.0007214102,0.0001191719,0.00023112688,0.0003786262,0.00019196374,0.001117928],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009847645,0.000030414523,0.9780904,0.000030780786,0.000035594145,0.00008009935,0.00021448848,0.00052052125,0.0060000317,0.00068143074,0.0040562097,0.010161546],"study_design_scores_gemma":[0.0000028298714,0.000009682873,0.9967303,0.0000027767967,0.0000055031774,0.000040748462,0.000020737129,0.00028510983,0.00044580334,0.00004139596,0.0024129613,0.0000020432683],"about_ca_topic_score_codex":0.009306337,"about_ca_topic_score_gemma":0.012763206,"teacher_disagreement_score":0.009306337,"about_ca_system_score_codex":0.00039302802,"about_ca_system_score_gemma":0.00020052139,"threshold_uncertainty_score":0.018504322},"labels":[],"label_agreement":null},{"id":"W1970219773","doi":"10.1086/497133","title":"Semianalytical Dark Matter Halos and the Jeans Equation","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Dark matter; Halo; Hydrostatic equilibrium; Asymptote; Power law; RADIUS; Statistical physics; Astrophysics; Isotropy; Scale (ratio); Classical mechanics; Mathematical analysis; Mathematics; Quantum mechanics; Statistics; Galaxy; Computer science","score_opus":0.007121595005787086,"score_gpt":0.2086839804825569,"score_spread":0.20156238547676983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970219773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86428756,0.00092561316,0.10270548,0.0009485951,0.000026036434,0.000024807252,0.00009288115,0.0002042494,0.030784816],"genre_scores_gemma":[0.9935348,0.00018936287,0.004711404,0.000039337327,0.00001570223,0.000007947309,0.000027460597,0.000021981177,0.0014519426],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990356,0.000033409495,0.000004189312,0.000010050022,0.000028073258,0.00002061869],"domain_scores_gemma":[0.99939966,0.00023456488,0.00018319467,0.00005859968,0.00006698921,0.00005698948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003610102,0.0002439484,0.00019085701,0.0005475521,0.0003038496,0.0008007468,0.0005150432,0.00025232238,0.0012011],"category_scores_gemma":[0.002834312,0.00016832165,0.00030091513,0.00023918874,0.0014246751,0.00082745287,0.00093645096,0.00033580634,0.00013785955],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000032696233,0.000028919394,0.005926426,0.000046498775,0.0000203814,0.00029792186,0.0003376481,0.19410862,0.004663525,0.78898585,0.0005994658,0.0049520284],"study_design_scores_gemma":[0.000017637163,0.000009337505,0.0036230893,0.000013176284,0.000005778678,0.00016406245,0.000097411554,0.7088648,0.0005377749,0.28511807,0.0015304286,0.000018402294],"about_ca_topic_score_codex":0.004780446,"about_ca_topic_score_gemma":0.002482776,"teacher_disagreement_score":0.004780446,"about_ca_system_score_codex":0.0008906034,"about_ca_system_score_gemma":0.00045958403,"threshold_uncertainty_score":0.009505212},"labels":[],"label_agreement":null},{"id":"W1970245236","doi":"10.1088/0004-637x/783/2/90","title":"HIGH-RESOLUTION SUBMILLIMETER AND NEAR-INFRARED STUDIES OF THE TRANSITION DISK AROUND Sz 91","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Smithsonian Astrophysical Observatory; Academia Sinica; Japan Society for the Promotion of Science; Ministry of Education, Culture, Sports, Science and Technology; Smithsonian Institution; National Science Foundation","keywords":"Submillimeter Array; Protoplanet; RADIUS; Spectral energy distribution; Debris disk; Stars; Thick disk; Circumstellar disk; Mass distribution","score_opus":0.011912191312799318,"score_gpt":0.23216968920858327,"score_spread":0.22025749789578394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970245236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999111,0.00008500572,0.00020546105,0.000007163878,0.0000015323576,0.0000028961856,0.0001126014,0.000010076766,0.00046423747],"genre_scores_gemma":[0.9988117,0.00007580657,0.00047204888,0.000015085538,0.000005876323,0.000003881124,0.00042669883,0.0000046247646,0.00018430126],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994445,0.0000032178366,0.0000028240156,0.000016407515,0.000014632445,0.000018358187],"domain_scores_gemma":[0.9998536,0.000014820732,0.00005311802,0.000012643182,0.000023285285,0.000042530577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008149313,0.00014375811,0.00020110385,0.0005508279,0.0002488512,0.00035740717,0.00024271324,0.00015183078,0.00056169985],"category_scores_gemma":[0.00014152561,0.00012978444,0.0001927355,0.0003602691,0.0001267403,0.00019640687,0.0003391236,0.00027224855,0.00026013263],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031056537,0.00009445182,0.3361951,0.000065905675,0.000052196476,0.0007456413,0.0006239491,0.000425142,0.64944214,0.00016129586,0.00018204293,0.011701635],"study_design_scores_gemma":[0.0000066725534,0.00005257041,0.99393713,0.0000025939164,0.000011288271,0.0002467913,0.00018220361,0.0003422964,0.0047573326,0.000024306999,0.00043341442,0.0000033231036],"about_ca_topic_score_codex":0.0020516533,"about_ca_topic_score_gemma":0.0032462396,"teacher_disagreement_score":0.0020516533,"about_ca_system_score_codex":0.0001905094,"about_ca_system_score_gemma":0.00006991282,"threshold_uncertainty_score":0.0040794015},"labels":[],"label_agreement":null},{"id":"W1970330643","doi":"10.1088/0004-637x/748/1/7","title":"THE ATACAMA COSMOLOGY TELESCOPE: ACT-CL J0102–4915 “EL GORDO,” A MASSIVE MERGING CLUSTER AT REDSHIFT 0.87","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":177,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Redshift; Cluster (spacecraft); Luminosity; Galaxy cluster; Sky; Galaxy; Surface brightness; Cosmology","score_opus":0.007514114335779782,"score_gpt":0.2279315825972903,"score_spread":0.2204174682615105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970330643","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7378809,0.00093703216,0.00460275,0.006207431,0.00081811013,0.00029789985,0.052798145,0.0024273808,0.19403027],"genre_scores_gemma":[0.90210706,0.00031128162,0.0097567765,0.0015872298,0.00038361026,0.000110624926,0.04412463,0.0005547666,0.04106408],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99966156,0.000034777313,0.000008608358,0.000094886804,0.00014223806,0.000057934474],"domain_scores_gemma":[0.99917525,0.000034884597,0.00012825575,0.00011292547,0.00021138601,0.00033724346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060880254,0.00022374466,0.0002746235,0.0014797964,0.0021202727,0.0010097321,0.0006158448,0.00052913715,0.0085151745],"category_scores_gemma":[0.0007880642,0.00021883739,0.00014309399,0.0016879603,0.0004971846,0.0010434461,0.0012407055,0.0008128153,0.0028930274],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009897071,0.00040635242,0.3505679,0.00025359693,0.00016690911,0.0014909595,0.0032168475,0.0009782886,0.021125926,0.017379379,0.5342093,0.06921481],"study_design_scores_gemma":[0.00015494016,0.00007123547,0.68908817,0.0000618298,0.000051056628,0.0004953685,0.0013397117,0.0035973273,0.0023069754,0.002558824,0.3002161,0.00005842539],"about_ca_topic_score_codex":0.08882388,"about_ca_topic_score_gemma":0.15734479,"teacher_disagreement_score":0.08882388,"about_ca_system_score_codex":0.0011975795,"about_ca_system_score_gemma":0.0013877571,"threshold_uncertainty_score":0.17661375},"labels":[],"label_agreement":null},{"id":"W1970360517","doi":"10.1086/510877","title":"The Planetary Mass Companion 2MASS 1207−3932B: Temperature, Mass, and Evidence for an Edge‐on Disk","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":175,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Photometry (optics); Primary (astronomy); Planetary mass; Spectral line; Effective temperature; Brown dwarf; Astronomy; Spectroscopy; Low Mass; Mass ratio; Planet; Planetary system","score_opus":0.026278743394486125,"score_gpt":0.2842661903885002,"score_spread":0.2579874469940141,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970360517","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947508,0.00017882268,0.00010198702,0.0000808388,0.000012022607,0.000010751773,0.00071649475,0.00003351073,0.0041148188],"genre_scores_gemma":[0.9951119,0.00007555192,0.00024281333,0.000050619794,0.000027850381,0.0000065663403,0.002949569,0.000011879067,0.0015232426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992144,0.0000035631856,0.0000028139364,0.00002271129,0.000027238479,0.0000221484],"domain_scores_gemma":[0.99980336,0.0000131577335,0.00005190587,0.000015970189,0.000028930635,0.00008656281],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000107557884,0.00036615942,0.0003680938,0.0011911086,0.0007388519,0.00051780994,0.0004932412,0.0005094832,0.0038508247],"category_scores_gemma":[0.00021538517,0.0001628005,0.00013599664,0.0008066188,0.00022610193,0.0002370268,0.0003334027,0.0003092796,0.0017785439],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004883027,0.000444111,0.8865947,0.00007302414,0.00007421153,0.0064565656,0.0009028338,0.0002748052,0.07383325,0.0007105918,0.009673998,0.020473653],"study_design_scores_gemma":[0.00002787021,0.00015360562,0.9852828,0.000010472601,0.000018741928,0.0044425097,0.00030103303,0.00080830196,0.0021216809,0.00025453107,0.00656804,0.00001036706],"about_ca_topic_score_codex":0.009395505,"about_ca_topic_score_gemma":0.014072153,"teacher_disagreement_score":0.009395505,"about_ca_system_score_codex":0.0004895878,"about_ca_system_score_gemma":0.00016370101,"threshold_uncertainty_score":0.018681645},"labels":[],"label_agreement":null},{"id":"W1970387030","doi":"10.1088/0004-637x/768/2/183","title":"GALACTIC ULTRACOMPACT X-RAY BINARIES: EMPIRICAL LUMINOSITIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Milky Way; Luminosity; Luminosity function; Bulge; Galaxy; Field (mathematics); Instability","score_opus":0.019379103127118037,"score_gpt":0.25733431827769077,"score_spread":0.23795521515057272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970387030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947148,0.0006941373,0.0021561896,0.0000335913,0.0000027436206,0.000007275922,0.00037029042,0.00004723905,0.0019737016],"genre_scores_gemma":[0.99878913,0.00018406683,0.00046338784,0.000009354203,0.0000071849868,0.0000047411168,0.0003461313,0.000011865001,0.00018416533],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979824,0.000032886117,0.000019331721,0.00007619828,0.00003945544,0.00003395033],"domain_scores_gemma":[0.99709094,0.0012843997,0.0007644752,0.00040138405,0.00021978516,0.00023901246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000517214,0.00032832907,0.00026656376,0.0015144271,0.00028625166,0.0012163422,0.0005295635,0.0003702247,0.0016831277],"category_scores_gemma":[0.0051121283,0.0001761719,0.00016740467,0.0009905607,0.0008870144,0.0012646297,0.00073478854,0.0004331754,0.00062137865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003895561,0.000015903135,0.99121726,0.000016226235,0.0000362424,0.000041967887,0.00012362252,0.0018648687,0.0009124295,0.0008496165,0.00010068265,0.004782284],"study_design_scores_gemma":[0.000005049399,0.00002711727,0.9821447,0.00001728024,0.000022042379,0.0004226873,0.00022876216,0.012188699,0.001568454,0.0025523333,0.00081203267,0.000010700512],"about_ca_topic_score_codex":0.0024318495,"about_ca_topic_score_gemma":0.0016583493,"teacher_disagreement_score":0.0024318495,"about_ca_system_score_codex":0.00048262265,"about_ca_system_score_gemma":0.000113205664,"threshold_uncertainty_score":0.0056306124},"labels":[],"label_agreement":null},{"id":"W1970440163","doi":"10.1086/427937","title":"Cosmic Star Formation History and Its Dependence on Galaxy Stellar Mass","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":357,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"COSMIC cancer database; Astrophysics; Star (game theory); Star formation; Astronomy; Galaxy; Physics; Stellar mass","score_opus":0.010044737457519366,"score_gpt":0.20056636431013436,"score_spread":0.190521626852615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970440163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99719125,0.00024261259,0.0001869899,0.000037665246,0.0000030477427,0.0000035691103,0.0009041017,0.000021888925,0.0014087716],"genre_scores_gemma":[0.999116,0.000057831556,0.000062278305,0.000004871928,0.0000049657065,0.000002106253,0.0005629073,0.0000048126844,0.00018411654],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974924,0.00005098958,0.000020381784,0.00006910532,0.000054600012,0.00005567897],"domain_scores_gemma":[0.9959823,0.0013412179,0.0015433525,0.0003420298,0.00025901946,0.00053199066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043046087,0.0002189361,0.00023399702,0.001612867,0.0001632689,0.00057060743,0.00024338598,0.0003249116,0.0019633782],"category_scores_gemma":[0.0036886553,0.00012579538,0.00035951086,0.0013719545,0.0002964168,0.00040559447,0.00038489263,0.00029316594,0.00043505707],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004734615,0.00000957347,0.99504375,0.000008203123,0.00005640244,0.00004605475,0.000099115096,0.0005480734,0.0008312846,0.00017308332,0.00009391173,0.0030430218],"study_design_scores_gemma":[7.7882197e-7,0.0000159534,0.9989219,0.0000020669574,0.000006591273,0.00005317116,0.000016174632,0.0006731067,0.000096495256,0.000040284755,0.0001714068,0.0000021394897],"about_ca_topic_score_codex":0.0061413944,"about_ca_topic_score_gemma":0.006064258,"teacher_disagreement_score":0.0061413944,"about_ca_system_score_codex":0.0002720703,"about_ca_system_score_gemma":0.00011663004,"threshold_uncertainty_score":0.012211323},"labels":[],"label_agreement":null},{"id":"W1970529252","doi":"10.1088/0004-637x/718/2/1158","title":"WHERE DO WET, DRY, AND MIXED GALAXY MERGERS OCCUR? A STUDY OF THE ENVIRONMENTS OF CLOSE GALAXY PAIRS IN THE DEEP2 GALAXY REDSHIFT SURVEY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Trent University","funders":"","keywords":"Galaxy merger; Astrophysics; Physics; Galaxy; Merge (version control); Redshift; Astronomy","score_opus":0.008231829302594373,"score_gpt":0.21606925907265295,"score_spread":0.2078374297700586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970529252","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995721,0.00008852491,0.000050829178,0.0000098338205,3.2123572e-7,0.0000011269611,0.000044356915,0.0000020810924,0.00023083093],"genre_scores_gemma":[0.99977416,0.000042857966,0.000038078226,0.0000039494525,0.0000014706225,7.249535e-7,0.00008044909,0.0000011161849,0.000057205485],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996563,0.00007974507,0.00001850381,0.00008669316,0.00005638451,0.00010241717],"domain_scores_gemma":[0.99840814,0.000279988,0.0007759146,0.0000925111,0.00009924216,0.00034423417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044676167,0.00018214052,0.0002817014,0.0010529708,0.00042481755,0.00080946,0.00026440618,0.00029505725,0.0007767247],"category_scores_gemma":[0.0019407887,0.000278508,0.00019326422,0.00096404913,0.00043759128,0.00097476615,0.0011010735,0.00023909366,0.00017866628],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008986246,0.000013660617,0.9948473,0.000006959735,0.00003535241,0.00011718877,0.00036053368,0.00027098873,0.0019830717,0.0002174428,0.000062001105,0.0019956804],"study_design_scores_gemma":[0.0000017061458,0.000016990103,0.9989127,0.0000012399672,0.000006542484,0.00009662025,0.00025984054,0.00036800996,0.00013022013,0.00004094238,0.00016266221,0.000002579382],"about_ca_topic_score_codex":0.0062338933,"about_ca_topic_score_gemma":0.0105518885,"teacher_disagreement_score":0.0062338933,"about_ca_system_score_codex":0.00033163856,"about_ca_system_score_gemma":0.000119059,"threshold_uncertainty_score":0.012395203},"labels":[],"label_agreement":null},{"id":"W1970544603","doi":"10.1088/0004-637x/803/2/75","title":"SIMULATING TIDAL STREAMS IN A HIGH-RESOLUTION DARK MATTER HALO","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Halo; Physics; STREAMS; Astrophysics; Dark matter halo; Dark matter; Cuspy halo problem; Redshift; Perturbation (astronomy); Astronomy; Galaxy","score_opus":0.010267890365949774,"score_gpt":0.22167907789880306,"score_spread":0.2114111875328533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970544603","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9902208,0.00008687703,0.005208627,0.00015901998,0.000022205371,0.000033232252,0.00038118413,0.00019257223,0.0036954866],"genre_scores_gemma":[0.9956417,0.00005771433,0.0032579692,0.00004883087,0.0000073120773,0.000021480264,0.00031127466,0.00004092984,0.00061264366],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988246,0.00004243882,0.0000047022304,0.000014724654,0.000017352464,0.000038355272],"domain_scores_gemma":[0.9993198,0.00025607797,0.00007258144,0.00007262049,0.000087706365,0.00019124158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004528232,0.00040579154,0.00042881237,0.00052755437,0.00043302428,0.0008505191,0.0010387003,0.00086843973,0.0013445049],"category_scores_gemma":[0.002278913,0.00033446698,0.00054042245,0.0006626428,0.0007694726,0.00057203334,0.00090521446,0.00049705117,0.000137123],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013768046,0.000061906896,0.008085521,0.000017060785,0.000034043514,0.00013937661,0.00007206792,0.9866484,0.001039241,0.002488285,0.00024933068,0.0010272054],"study_design_scores_gemma":[0.00007930894,0.00003484417,0.0014634823,0.0000037081682,0.000009137882,0.000015185231,0.000040970026,0.99695385,0.00035154467,0.00078750047,0.00025243105,0.000008004679],"about_ca_topic_score_codex":0.028521635,"about_ca_topic_score_gemma":0.012441038,"teacher_disagreement_score":0.028521635,"about_ca_system_score_codex":0.0010101714,"about_ca_system_score_gemma":0.0009847254,"threshold_uncertainty_score":0.056711197},"labels":[],"label_agreement":null},{"id":"W1970622085","doi":"10.1088/0004-637x/696/2/1084","title":"<i>FERMI</i>LARGE AREA TELESCOPE OBSERVATIONS OF THE VELA PULSAR","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":139,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Vela; Physics; Pulsar; Astrophysics; Fermi Gamma-ray Space Telescope; Nebula; Astronomy; Telescope; Magnetosphere; Sky; Stars; Plasma; Nuclear physics","score_opus":0.021176898556746183,"score_gpt":0.30309529742812585,"score_spread":0.28191839887137965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970622085","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9779123,0.0013105986,0.0048953653,0.0004765961,0.00003834295,0.000018813462,0.0027281118,0.00039744607,0.012222421],"genre_scores_gemma":[0.9903803,0.00023328922,0.0051172003,0.00010605587,0.000059644655,0.000011189471,0.0026644242,0.00004425884,0.0013837295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991655,0.000012492406,0.000004261554,0.000017225042,0.000026114047,0.000023381883],"domain_scores_gemma":[0.9996661,0.0000767051,0.00006602676,0.00008155923,0.0000566187,0.000053039526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035911662,0.0001257702,0.00009969902,0.0011829704,0.0005459769,0.0005226172,0.0002448549,0.00020196916,0.0014093602],"category_scores_gemma":[0.0006397829,0.0001311243,0.00018342008,0.00067267974,0.00021602541,0.0002599246,0.00047884104,0.00031076602,0.00025955588],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006593795,0.0002152,0.57315546,0.00021010224,0.00030164374,0.0014736,0.0007542277,0.004405886,0.24630803,0.0037966913,0.015055761,0.15366392],"study_design_scores_gemma":[0.00002381978,0.00007727869,0.9788285,0.000029287992,0.0000506604,0.00060230086,0.00005108842,0.0015627698,0.009235722,0.0006154215,0.008904989,0.000018128723],"about_ca_topic_score_codex":0.004593979,"about_ca_topic_score_gemma":0.01057195,"teacher_disagreement_score":0.004593979,"about_ca_system_score_codex":0.00036534405,"about_ca_system_score_gemma":0.00018433388,"threshold_uncertainty_score":0.009134471},"labels":[],"label_agreement":null},{"id":"W1970658634","doi":"10.1086/429860","title":"On the Dynamics of Suddenly Heated Accretion Disks around Neutron Stars","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Accretion (finance); Neutron star; Outflow; Radiative transfer; Angular momentum; Inflow; Accretion disc; Intermediate polar; Black-body radiation","score_opus":0.012836227822482242,"score_gpt":0.23564107897270156,"score_spread":0.2228048511502193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970658634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99450004,0.00027263968,0.0013506255,0.00009540199,0.000019344161,0.0000102190015,0.00008023133,0.00003698433,0.0036345373],"genre_scores_gemma":[0.9986168,0.00016613377,0.00026792756,0.000016476208,0.000010873235,0.0000058062797,0.00008235685,0.000016086557,0.00081754534],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994755,0.000009936708,0.0000027205735,0.000010748262,0.000010878404,0.000018195153],"domain_scores_gemma":[0.99976534,0.00005623566,0.000078880934,0.000017007995,0.000026399486,0.00005601076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012775687,0.00036642724,0.00036420568,0.00037413414,0.0005092446,0.00060461886,0.00043869374,0.00036876887,0.0022511445],"category_scores_gemma":[0.00069925055,0.00021172379,0.00038543827,0.00018570285,0.0005199634,0.00046879277,0.00065304426,0.00030946985,0.00033428878],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016353941,0.00025178783,0.13122874,0.00023297375,0.00032056798,0.006827679,0.0010784655,0.71960783,0.09818376,0.016685467,0.0016873359,0.022259984],"study_design_scores_gemma":[0.00011850683,0.00026373882,0.14703667,0.00004523819,0.00007736401,0.00054285134,0.00047912265,0.83579654,0.0076871044,0.005592696,0.0022945222,0.000065785345],"about_ca_topic_score_codex":0.00452093,"about_ca_topic_score_gemma":0.0027645323,"teacher_disagreement_score":0.00452093,"about_ca_system_score_codex":0.0007396685,"about_ca_system_score_gemma":0.00021271895,"threshold_uncertainty_score":0.008989215},"labels":[],"label_agreement":null},{"id":"W1970671876","doi":"10.1088/0004-637x/775/1/69","title":"STELLAR DYNAMOS AND CYCLES FROM NUMERICAL SIMULATIONS OF CONVECTION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Dynamo; Convection; Astrophysics; Dynamo theory; Computational astrophysics; Astronomy; Stellar wind; Mechanics; Stars; Classical mechanics; Magnetic field","score_opus":0.00521289430259636,"score_gpt":0.21391455021824682,"score_spread":0.20870165591565046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970671876","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98158836,0.00015454643,0.011574736,0.0001697597,0.00002339963,0.000030969804,0.0002658277,0.00013078528,0.00606155],"genre_scores_gemma":[0.99608,0.00008798307,0.0031137604,0.000021278647,0.000010669843,0.000036341648,0.00017526097,0.00003797104,0.00043669346],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992645,0.00002337061,0.000006073909,0.000010713772,0.000017142225,0.00001620208],"domain_scores_gemma":[0.9996151,0.00018145399,0.0000770091,0.000038831367,0.00003572431,0.000051858842],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032476668,0.0004081855,0.0003278158,0.00047857294,0.00032346608,0.00056051224,0.00043769434,0.0004713365,0.00088034576],"category_scores_gemma":[0.0015581991,0.000248808,0.00040366486,0.00035865014,0.00056891306,0.0004002952,0.0006055122,0.00038960925,0.00007939777],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054816737,0.000030914267,0.0059146695,0.000028415667,0.000023908387,0.000061191284,0.00009176654,0.98481005,0.0016223829,0.004800015,0.00018448112,0.0023774025],"study_design_scores_gemma":[0.000012706823,0.000011370787,0.0006533604,0.0000030433882,0.0000033112913,0.0000081862445,0.000010695465,0.99763143,0.00027954378,0.001205893,0.00017705567,0.0000033404367],"about_ca_topic_score_codex":0.0048348443,"about_ca_topic_score_gemma":0.0030032562,"teacher_disagreement_score":0.0048348443,"about_ca_system_score_codex":0.00057168555,"about_ca_system_score_gemma":0.00044624944,"threshold_uncertainty_score":0.009613395},"labels":[],"label_agreement":null},{"id":"W1970693245","doi":"10.1086/379010","title":"<i>Chandra</i>Observation of the Edge‐on Galaxy NGC 3556 (M108): Violent Galactic Disk‐Halo Interaction Revealed","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Astronomy; Halo; Galaxy; Spiral galaxy; Barred spiral galaxy; Galactic halo; Supernova; Galaxy merger; Star formation","score_opus":0.016231150948094696,"score_gpt":0.24034692510763253,"score_spread":0.22411577415953784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970693245","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99687517,0.00016977091,0.00013686616,0.000050535262,0.000009818499,0.000009518703,0.00081851153,0.00009270918,0.0018370623],"genre_scores_gemma":[0.9971781,0.000075810516,0.0009318342,0.00005022711,0.00001684719,0.0000058565934,0.0012213876,0.000012963641,0.0005068832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999442,0.0000030326366,0.000003583482,0.000014416334,0.0000143995985,0.000020303627],"domain_scores_gemma":[0.999798,0.000011218469,0.00004704729,0.000023497356,0.000013759765,0.00010647066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000071720126,0.00025736712,0.00020373017,0.00074316515,0.0003604811,0.0003076451,0.00027404755,0.00028802012,0.0012900309],"category_scores_gemma":[0.00015521988,0.0001454204,0.00022613857,0.00044234475,0.00016721578,0.000201628,0.00050609803,0.0003166388,0.0003090435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012793338,0.00025818424,0.50636756,0.0002828272,0.00019517151,0.00622224,0.0013541904,0.0008863356,0.44902363,0.0006942281,0.00420244,0.02923383],"study_design_scores_gemma":[0.000021745083,0.00019008708,0.98722804,0.00001732438,0.00003765852,0.0025915296,0.0001459127,0.00043668068,0.005106783,0.000108214306,0.0041028927,0.000013029215],"about_ca_topic_score_codex":0.0049022874,"about_ca_topic_score_gemma":0.011547004,"teacher_disagreement_score":0.0049022874,"about_ca_system_score_codex":0.00020188809,"about_ca_system_score_gemma":0.000117188334,"threshold_uncertainty_score":0.009747505},"labels":[],"label_agreement":null},{"id":"W1970702820","doi":"10.1088/0004-637x/768/2/121","title":"<i>HST</i>SPECTRAL MAPPING OF L/T TRANSITION BROWN DWARFS REVEALS CLOUD THICKNESS VARIATIONS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":225,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Brightness; Surface brightness; Stellar classification; Infrared; Massive compact halo object; Radiative transfer; Molecular cloud","score_opus":0.01142620669543041,"score_gpt":0.2130451035277351,"score_spread":0.2016188968323047,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970702820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99612325,0.00006929532,0.0015819911,0.000020532787,0.000002740207,0.0000024691035,0.0005391128,0.00018450733,0.001476101],"genre_scores_gemma":[0.99752957,0.000032837794,0.0014599315,0.00001550788,0.0000039413976,0.0000016044504,0.0006250177,0.0000133165595,0.0003183463],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999789,0.0000017769227,0.0000011016132,0.000008863752,0.0000058200744,0.0000035587038],"domain_scores_gemma":[0.99992454,0.0000062611716,0.000027086195,0.000012325646,0.000011488151,0.000018357803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059087106,0.0001168362,0.00006749608,0.00041088418,0.00010772416,0.0002203461,0.00009514044,0.00009314584,0.00074698933],"category_scores_gemma":[0.00009983678,0.00005212964,0.00009905794,0.0002657064,0.00010710754,0.00009925584,0.000093341456,0.00008440602,0.00023504616],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016945852,0.00004389042,0.4346944,0.000049932827,0.00004659434,0.00026908933,0.00020039901,0.004400951,0.5333715,0.0007991455,0.0012929771,0.024661656],"study_design_scores_gemma":[0.0000039638967,0.000037957994,0.9722077,0.0000025354327,0.000010604205,0.00022975761,0.00006451849,0.0084022,0.017671738,0.00022324112,0.0011404668,0.000005243528],"about_ca_topic_score_codex":0.0029966144,"about_ca_topic_score_gemma":0.004807368,"teacher_disagreement_score":0.0029966144,"about_ca_system_score_codex":0.00015479495,"about_ca_system_score_gemma":0.000058403773,"threshold_uncertainty_score":0.0059583783},"labels":[],"label_agreement":null},{"id":"W1970792124","doi":"10.1088/0004-637x/758/1/6","title":"NOISE IN THE CROSS-POWER SPECTRUM OF THE VELA PULSAR","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Gaussian noise; Pulsar; Noise (video); Scintillation; Spectral density; Noise spectral density; Optics; Acoustics; Astrophysics; Noise figure; Statistics; Mathematics; Detector; Algorithm","score_opus":0.011527615179328852,"score_gpt":0.3244945685818336,"score_spread":0.31296695340250474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970792124","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9327501,0.00038915468,0.060905825,0.00028651094,0.00004389537,0.000018477194,0.00039979257,0.0005189696,0.004687217],"genre_scores_gemma":[0.9947248,0.0001237766,0.004153389,0.00003843195,0.00003487392,0.000010994056,0.0005174951,0.000087083965,0.00030912927],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995647,0.000096719465,0.000019174935,0.0001122705,0.00015420892,0.000052952728],"domain_scores_gemma":[0.99744105,0.0017002515,0.0002791167,0.00024215298,0.0002475831,0.00008988194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011715423,0.0004612276,0.00023462834,0.0015107645,0.00030182512,0.0007681751,0.00040821216,0.0003941728,0.0009146162],"category_scores_gemma":[0.0069861785,0.00020020064,0.00031361138,0.0011787696,0.0005749727,0.00073096505,0.0006230797,0.0005177282,0.00029761097],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001438506,0.00040588525,0.32068315,0.00038755705,0.0004714408,0.0021675362,0.0011098228,0.28282964,0.20373203,0.043801736,0.0033724906,0.13960038],"study_design_scores_gemma":[0.000047764548,0.00024025668,0.3107529,0.000064426546,0.00011996835,0.0012065212,0.00012635511,0.62413937,0.0435216,0.016761096,0.002889178,0.00013054135],"about_ca_topic_score_codex":0.0009687736,"about_ca_topic_score_gemma":0.0008056808,"teacher_disagreement_score":0.0015107645,"about_ca_system_score_codex":0.000487742,"about_ca_system_score_gemma":0.00018294012,"threshold_uncertainty_score":0.0061957836},"labels":[],"label_agreement":null},{"id":"W1970800496","doi":"10.1088/0004-637x/785/2/163","title":"THE FINAL-PARSEC PROBLEM IN NONSPHERICAL GALAXIES REVISITED","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Binary number; Extrapolation; Galaxy; Stars; Binary star; Supermassive black hole; Limiting; Binary black hole","score_opus":0.008362059124308383,"score_gpt":0.2115553722507333,"score_spread":0.2031933131264249,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970800496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88345486,0.00082736806,0.0928274,0.0036976843,0.000092978655,0.000054695938,0.0011489914,0.0007268833,0.017169062],"genre_scores_gemma":[0.9745768,0.00034130542,0.020945517,0.00037713407,0.00006797097,0.00006477681,0.0010111182,0.0002944429,0.0023210628],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996338,0.00014756533,0.000010885927,0.00006128238,0.000056399425,0.00009011648],"domain_scores_gemma":[0.99701786,0.0018420483,0.00035309375,0.0002972769,0.00022797946,0.00026169998],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002114531,0.0006460749,0.0009204092,0.00082534447,0.0017196906,0.0019864095,0.0021555813,0.0013550739,0.0033896223],"category_scores_gemma":[0.013121858,0.0004988884,0.00088702666,0.00085217314,0.002395102,0.0028618851,0.0015618162,0.0020253295,0.000392585],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016057656,0.00014224912,0.04335524,0.0000994803,0.0000874101,0.00072425103,0.0010499335,0.7153691,0.00080998056,0.22237033,0.0041739563,0.011657443],"study_design_scores_gemma":[0.00004888309,0.000033273976,0.010478827,0.000031231993,0.000021027323,0.00021765023,0.00033353514,0.88462186,0.00056055025,0.10105793,0.0025641418,0.0000310508],"about_ca_topic_score_codex":0.027010988,"about_ca_topic_score_gemma":0.016063547,"teacher_disagreement_score":0.027010988,"about_ca_system_score_codex":0.0018132086,"about_ca_system_score_gemma":0.0015021325,"threshold_uncertainty_score":0.05370754},"labels":[],"label_agreement":null},{"id":"W1970841187","doi":"10.1088/0004-637x/774/1/23","title":"THE GROWTH OF COOL CORES AND EVOLUTION OF COOLING PROPERTIES IN A SAMPLE OF 83 GALAXY CLUSTERS AT 0.3 &lt;<i>z</i>&lt; 1.2 SELECTED FROM THE SPT-SZ SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":203,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"Argonne National Laboratory; Space Telescope Science Institute; University of Chicago; Smithsonian Astrophysical Observatory; U.S. Department of Energy; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; Surface brightness; Galaxy cluster; Cooling flow; Redshift; Cluster (spacecraft); Galaxy","score_opus":0.009516682329396729,"score_gpt":0.18874472081317883,"score_spread":0.1792280384837821,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970841187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942756,0.000050214312,0.000014512426,0.000011725037,5.1924275e-7,0.0000012199326,0.0003255171,0.0000028382194,0.0001659219],"genre_scores_gemma":[0.99905735,0.000036187525,0.000023688963,0.0000069270905,0.000002253298,0.000002559152,0.0005823041,0.0000027797676,0.00028600288],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989915,0.000010478576,0.0000064881715,0.000031726835,0.000015105707,0.000037101945],"domain_scores_gemma":[0.998801,0.00015151664,0.0005305868,0.00007870061,0.00016100814,0.00027722327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021990159,0.00009718303,0.00017659202,0.0014080448,0.00042329603,0.0005843677,0.0002650915,0.0001952211,0.0013812181],"category_scores_gemma":[0.0011554484,0.00014927909,0.00012715235,0.0010933909,0.00034823405,0.00031939658,0.00074825436,0.00019974589,0.00033357536],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009606157,0.0000142526615,0.9959604,0.0000060519064,0.000016081663,0.000029069188,0.0004466865,0.00007188143,0.001195699,0.000060845145,0.00019348296,0.0019095337],"study_design_scores_gemma":[6.0969313e-7,0.000005061125,0.99975055,5.366891e-7,0.0000017686158,0.000014308101,0.00009771119,0.000032319906,0.000025690726,0.0000051124935,0.00006567794,6.225062e-7],"about_ca_topic_score_codex":0.026734812,"about_ca_topic_score_gemma":0.046926107,"teacher_disagreement_score":0.026734812,"about_ca_system_score_codex":0.00036608998,"about_ca_system_score_gemma":0.00021139056,"threshold_uncertainty_score":0.053158343},"labels":[],"label_agreement":null},{"id":"W1970860842","doi":"10.1086/518711","title":"A New Model for the Loop I (North Polar Spur) Region","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":146,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Herzberg Institute of Astrophysics","funders":"","keywords":"Polarization (electrochemistry); Spur; Polar; Physics; Protein filament; Sky; Loop (graph theory); Synchrotron; Astrophysics; Shell (structure); Optics; Astronomy; Materials science; Geology; Chemistry; Paleontology","score_opus":0.015986097768796417,"score_gpt":0.2347582185277421,"score_spread":0.21877212075894567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970860842","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.19430052,0.001100888,0.18725598,0.013788033,0.0016510044,0.00015583668,0.00089237175,0.0009959703,0.5998594],"genre_scores_gemma":[0.917919,0.00034265348,0.011879092,0.00072614534,0.0003013439,0.00006596292,0.00034958587,0.0002076062,0.06820854],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999856,0.00003170405,0.0000029531998,0.00004070019,0.000028280765,0.000040311657],"domain_scores_gemma":[0.99966943,0.00006329305,0.000039302668,0.00005119785,0.000084875464,0.00009185289],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027182035,0.00024246876,0.00038706855,0.00029155178,0.00094192155,0.0016057664,0.00090714026,0.0011162848,0.02639787],"category_scores_gemma":[0.0012974056,0.00016523394,0.00048814228,0.0002699209,0.0007045634,0.0019884582,0.0007569333,0.00066918874,0.0029807396],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015155274,0.000029121778,0.0025441924,0.000074633695,0.00002115053,0.00039738716,0.0004484727,0.052807707,0.002708284,0.8997927,0.02052128,0.020503582],"study_design_scores_gemma":[0.00019388214,0.00010465343,0.002281493,0.000042866,0.000034481167,0.00039176663,0.0005368598,0.1472107,0.0010858863,0.7649013,0.08317174,0.000044425477],"about_ca_topic_score_codex":0.0052868305,"about_ca_topic_score_gemma":0.0028953748,"teacher_disagreement_score":0.02639787,"about_ca_system_score_codex":0.0006656808,"about_ca_system_score_gemma":0.00076147635,"threshold_uncertainty_score":0.088309705},"labels":[],"label_agreement":null},{"id":"W1970879469","doi":"10.1088/0004-637x/771/1/12","title":"PRIMORDIAL GRAVITATIONAL WAVE DETECTABILITY WITH DEEP SMALL-SKY COSMIC MICROWAVE BACKGROUND EXPERIMENTS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Planck; Gravitational wave; Cosmic background radiation; Astrophysics; Sky; Pixel; Optics","score_opus":0.01424634785079999,"score_gpt":0.24008841746907994,"score_spread":0.22584206961827996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970879469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9489202,0.00009880003,0.047755178,0.0002539524,0.000010273024,0.000028281427,0.00036348565,0.0002043412,0.0023654425],"genre_scores_gemma":[0.9926139,0.000025361483,0.006888357,0.0000338493,0.0000049788214,0.00001416177,0.00021024095,0.000022552884,0.0001865476],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994822,0.00025153926,0.00001784183,0.00011267278,0.00006088463,0.00007483434],"domain_scores_gemma":[0.9938706,0.0044197724,0.000652872,0.0005664613,0.00025928454,0.00023107782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0036331683,0.0003834672,0.0005083801,0.0003923162,0.00030996444,0.00089930417,0.00082804676,0.0006197096,0.0009988276],"category_scores_gemma":[0.011358539,0.0002634889,0.00061867805,0.000435751,0.0012111963,0.0013989293,0.0009240567,0.00071607885,0.00009361663],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078360306,0.00013838237,0.06286066,0.00007238713,0.00017361142,0.00012213216,0.00013559972,0.89622635,0.0034749187,0.025399135,0.00067289505,0.009940326],"study_design_scores_gemma":[0.00011463254,0.00013521113,0.013695527,0.000012749671,0.000036180216,0.000031145424,0.000031863678,0.97030354,0.0022014969,0.013035801,0.0003695337,0.000032309792],"about_ca_topic_score_codex":0.007609397,"about_ca_topic_score_gemma":0.004395524,"teacher_disagreement_score":0.007609397,"about_ca_system_score_codex":0.00071946066,"about_ca_system_score_gemma":0.0004200447,"threshold_uncertainty_score":0.019214272},"labels":[],"label_agreement":null},{"id":"W1970949801","doi":"10.1088/0004-637x/706/2/1277","title":"STRÖMGREN PHOTOMETRY OF GALACTIC GLOBULAR CLUSTERS. II. METALLICITY DISTRIBUTION OF RED GIANTS IN ω CENTAURI","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Metallicity; Physics; Globular cluster; Astrophysics; Photometry (optics); Stars; Astronomy; Open cluster; Star cluster","score_opus":0.009907259666376487,"score_gpt":0.23557576498383317,"score_spread":0.2256685053174567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1970949801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965934,0.0005043173,0.00029468274,0.000013774873,0.000004396785,0.000006413338,0.0007753046,0.000064087064,0.0017436495],"genre_scores_gemma":[0.9975452,0.00019923605,0.00036353114,0.000008976389,0.000007909897,0.0000088535635,0.0013312375,0.000012399685,0.00052251527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984705,0.000015010989,0.000013089022,0.00005146211,0.000036367863,0.00003700379],"domain_scores_gemma":[0.9995435,0.0000669087,0.00013795077,0.0000526879,0.00005518718,0.00014370847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002857042,0.0003780565,0.00023573224,0.0036022337,0.00032105405,0.0007147129,0.00025770083,0.00018628544,0.0014637691],"category_scores_gemma":[0.00068783545,0.00015285356,0.0002018873,0.0011587683,0.00035660583,0.00025534045,0.0007838025,0.00013279225,0.00066015485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013649874,0.000010978348,0.97148263,0.000046581976,0.000042730982,0.00010505121,0.00053081574,0.00039935907,0.012124912,0.0002780944,0.0004696911,0.014372629],"study_design_scores_gemma":[0.0000020051448,0.0000118526195,0.99865305,0.0000048030374,0.000008985064,0.00007814445,0.00007869404,0.0001494603,0.00039598468,0.00006386059,0.00055008294,0.0000029556193],"about_ca_topic_score_codex":0.0038760058,"about_ca_topic_score_gemma":0.007131936,"teacher_disagreement_score":0.0038760058,"about_ca_system_score_codex":0.00051870255,"about_ca_system_score_gemma":0.00010457738,"threshold_uncertainty_score":0.0077068806},"labels":[],"label_agreement":null},{"id":"W1971014996","doi":"10.1086/503861","title":"Mid‐Infrared Identifications of SCUBA Galaxies in the CUDSS 14 Hour Field with the<i>Spitzer Space Telescope</i>","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Spitzer Space Telescope; Physics; Galaxy; Astrophysics; Active galactic nucleus; Infrared; Star formation; Luminous infrared galaxy; Astronomy; Telescope; Population; Panchromatic film; Image resolution; Optics","score_opus":0.005199295072817482,"score_gpt":0.20027946158449234,"score_spread":0.19508016651167484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971014996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998896,0.000027957569,0.000043805103,0.000008405816,0.0000017077987,0.000004590413,0.00012672477,0.000010380906,0.00088050496],"genre_scores_gemma":[0.99861395,0.00003225528,0.00032856458,0.000014285715,0.0000072919356,0.000011117676,0.0006562689,0.0000026682294,0.00033352806],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997563,0.000022413642,0.000013477837,0.000047119236,0.00007089575,0.00008981477],"domain_scores_gemma":[0.998393,0.00014948953,0.0005444782,0.00018189862,0.00031604766,0.0004151277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028025024,0.0002371559,0.00018205891,0.0029135465,0.0007724447,0.00056331255,0.00042356926,0.00016499826,0.0014128267],"category_scores_gemma":[0.0009559141,0.0001555724,0.00014296005,0.0013514066,0.00048996427,0.0002549296,0.00069963216,0.00014772856,0.0002867715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001810601,0.000059506558,0.98115367,0.000012739271,0.000021062962,0.00022407823,0.00043218723,0.00012846127,0.0073705246,0.0001606858,0.0006518639,0.009604143],"study_design_scores_gemma":[0.0000058457395,0.000022923452,0.9985454,0.0000038953203,0.0000051735483,0.00010167619,0.00017386909,0.00018286535,0.00038969517,0.00003201929,0.0005340484,0.0000026831287],"about_ca_topic_score_codex":0.02112296,"about_ca_topic_score_gemma":0.042948626,"teacher_disagreement_score":0.02112296,"about_ca_system_score_codex":0.0006135549,"about_ca_system_score_gemma":0.0003053949,"threshold_uncertainty_score":0.042000055},"labels":[],"label_agreement":null},{"id":"W1971090960","doi":"10.1086/533424","title":"The Infrared Spectra of Very Large, Compact, Highly Symmetric, Polycyclic Aromatic Hydrocarbons (PAHs)","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":192,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Spectral line; Infrared; Wavelength; Spectral bands; Infrared spectroscopy; Analytical Chemistry (journal); Cationic polymerization","score_opus":0.010815905682862652,"score_gpt":0.22602598452336314,"score_spread":0.2152100788405005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971090960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9096896,0.0005653529,0.07404333,0.00010757614,0.000042424035,0.000029384337,0.0013802127,0.00037029112,0.013771874],"genre_scores_gemma":[0.97856575,0.0002468414,0.01788839,0.000024827814,0.000004636232,0.000018762064,0.00082173623,0.000034239878,0.0023947747],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99994135,0.0000054748457,0.0000012472495,0.000009813297,0.00003023657,0.000011861664],"domain_scores_gemma":[0.99990857,0.00004361616,0.000009643479,0.000010114436,0.000019458103,0.0000086037135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000118224205,0.00019859808,0.00018503898,0.0003863408,0.00022023037,0.00016823708,0.00029215976,0.00022749734,0.0035668653],"category_scores_gemma":[0.0003030153,0.0001241111,0.00034241387,0.00047041773,0.00022776234,0.00034524134,0.00018529165,0.00040241022,0.00051645294],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000394289,0.00021234746,0.01934035,0.0007757723,0.0001299756,0.00061685377,0.00030025488,0.1395338,0.7228295,0.015569279,0.0021871263,0.09811046],"study_design_scores_gemma":[0.000051056235,0.0005408097,0.08510004,0.000043827633,0.00007085105,0.0009392502,0.0006519487,0.5796808,0.30477202,0.015188483,0.01282153,0.00013935874],"about_ca_topic_score_codex":0.0011462386,"about_ca_topic_score_gemma":0.0016889466,"teacher_disagreement_score":0.0035668653,"about_ca_system_score_codex":0.00021403343,"about_ca_system_score_gemma":0.00019346407,"threshold_uncertainty_score":0.011932313},"labels":[],"label_agreement":null},{"id":"W1971157431","doi":"10.1088/0004-637x/728/1/69","title":"THE SURFACE OF V410 TAURI","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University","funders":"","keywords":"Physics; Astrophysics; Photosphere; Longitude; Amplitude; Polar; T Tauri star; Starspot; Latitude; Doppler effect; Astronomy; Light curve; Spectral line; Stars; Optics","score_opus":0.01644440510645555,"score_gpt":0.2165636575624211,"score_spread":0.20011925245596554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971157431","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967847,0.00014494499,0.00014981841,0.000021597227,0.0000060984735,0.0000027593164,0.00017905932,0.000018245823,0.002692888],"genre_scores_gemma":[0.99796665,0.00010324349,0.00043023206,0.000023033703,0.000008095536,0.0000036783838,0.0008015823,0.000014509383,0.0006491059],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994886,0.0000029181717,0.0000013891785,0.00001539113,0.000011231981,0.00002022445],"domain_scores_gemma":[0.99995506,0.0000056303093,0.000009299592,0.000006455581,0.0000101475825,0.000013365283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000045204117,0.00016951191,0.00011064715,0.00043623935,0.00030108818,0.00037463862,0.00014902295,0.00032372185,0.0012612604],"category_scores_gemma":[0.00014257059,0.00010224758,0.00014753781,0.00031773592,0.00012688612,0.0001484994,0.00026795297,0.00014656958,0.00043337734],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007411369,0.00008367159,0.17737722,0.00012278723,0.000052227388,0.0014983261,0.0009338564,0.0017562578,0.7832399,0.0005006907,0.0014809809,0.03221294],"study_design_scores_gemma":[0.000020381201,0.00018238406,0.9554133,0.000015467112,0.000027003125,0.0013849149,0.00049784314,0.0049448004,0.029356329,0.00018027968,0.007962001,0.000015343147],"about_ca_topic_score_codex":0.0029904651,"about_ca_topic_score_gemma":0.002084235,"teacher_disagreement_score":0.0029904651,"about_ca_system_score_codex":0.00022782576,"about_ca_system_score_gemma":0.00006130389,"threshold_uncertainty_score":0.0059460998},"labels":[],"label_agreement":null},{"id":"W1971179945","doi":"10.1088/0004-637x/736/2/78","title":"BROADBAND TRANSMISSION SPECTROSCOPY OF THE SUPER-EARTH GJ 1214b SUGGESTS A LOW MEAN MOLECULAR WEIGHT ATMOSPHERE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Transit (satellite); Absorption (acoustics); Optical depth; Spectroscopy; Scale height; Atmosphere (unit); Broadband; Spectral line","score_opus":0.0070266812358871,"score_gpt":0.19924154641229205,"score_spread":0.19221486517640496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971179945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99817014,0.000034250304,0.00015372789,0.000017569984,0.0000018136406,0.0000032142104,0.00022812499,0.000049822207,0.001341329],"genre_scores_gemma":[0.9989955,0.000021748605,0.00020548863,0.000011419362,0.0000018742222,0.0000029644477,0.000500562,0.000008968453,0.0002514369],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991345,0.000004115552,0.0000034736463,0.000022770879,0.00002850402,0.000027742819],"domain_scores_gemma":[0.99983025,0.0000198808,0.00005685641,0.000022194163,0.000032901917,0.000037865433],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000103131126,0.00029606998,0.00025364658,0.00083926076,0.00047610115,0.0004765241,0.00029330797,0.00035777793,0.001969563],"category_scores_gemma":[0.00030962864,0.00022185997,0.00016635985,0.0006825855,0.00022573229,0.00048265944,0.0004081046,0.00035122776,0.00036759707],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055512623,0.00012329334,0.41188154,0.00011534333,0.00011160284,0.0010831908,0.0005940251,0.0023870436,0.57056916,0.0007185416,0.001487698,0.010373384],"study_design_scores_gemma":[0.000013964383,0.000077858254,0.9864065,0.0000050952335,0.000027009779,0.00017868786,0.00013289836,0.0015982519,0.010294773,0.00008422684,0.0011709592,0.00000990395],"about_ca_topic_score_codex":0.008083106,"about_ca_topic_score_gemma":0.014665287,"teacher_disagreement_score":0.008083106,"about_ca_system_score_codex":0.00056191185,"about_ca_system_score_gemma":0.00011993411,"threshold_uncertainty_score":0.016072094},"labels":[],"label_agreement":null},{"id":"W1971180328","doi":"10.1088/0004-637x/772/1/7","title":"MEASUREMENT OF THE RADIUS OF NEUTRON STARS WITH HIGH SIGNAL-TO-NOISE QUIESCENT LOW-MASS X-RAY BINARIES IN GLOBULAR CLUSTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":227,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"RADIUS; Globular cluster; Neutron star; Spectral line; Range (aeronautics); Stars; Equation of state; Nucleosynthesis","score_opus":0.00801172076306432,"score_gpt":0.18810516244151052,"score_spread":0.1800934416784462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971180328","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99455583,0.000069169066,0.0050102132,0.0000064350133,0.0000011185566,0.0000044993435,0.000041393705,0.000034702327,0.00027668758],"genre_scores_gemma":[0.99870217,0.000014564914,0.0011602648,0.0000029804162,0.0000015097878,0.000002251337,0.000079975354,0.000004425578,0.000031903266],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995888,0.000076857184,0.000030099714,0.00015844677,0.00011289724,0.000032966233],"domain_scores_gemma":[0.99862564,0.00048699576,0.00043702795,0.00017326215,0.000117629585,0.00015953911],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010296436,0.00028239406,0.0002970038,0.00074914156,0.0004021406,0.00061119435,0.00062594324,0.00037337697,0.00021674589],"category_scores_gemma":[0.0042517497,0.00026821907,0.00020286157,0.0004290279,0.00051325763,0.00045764667,0.0010232944,0.00019893808,0.00011679566],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000376685,0.00003697152,0.88367486,0.000050094073,0.000095939264,0.00015210599,0.00052882824,0.04303437,0.06128412,0.0011048426,0.00005737549,0.009603708],"study_design_scores_gemma":[0.000017399945,0.00017718448,0.82736737,0.000016747877,0.00006217655,0.0004830558,0.00018751714,0.14546774,0.024776567,0.00093512516,0.00045012595,0.00005901192],"about_ca_topic_score_codex":0.0032224688,"about_ca_topic_score_gemma":0.0036289918,"teacher_disagreement_score":0.0032224688,"about_ca_system_score_codex":0.00050324923,"about_ca_system_score_gemma":0.00018112772,"threshold_uncertainty_score":0.0064074397},"labels":[],"label_agreement":null},{"id":"W1971196682","doi":"10.1086/524404","title":"Toward a Solution for the Ca <scp>ii</scp> Triplet Puzzle: Results from Dwarf Elliptical Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Nautical Research Society","funders":"","keywords":"Astrophysics; Metallicity; Physics; Photometry (optics); Spectroscopy; Stars; Galaxy; Star formation; Astronomy","score_opus":0.0281794154537733,"score_gpt":0.2824453680556637,"score_spread":0.25426595260189044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971196682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952348,0.0006482062,0.0014499814,0.00061874953,0.000006903956,0.0000067578817,0.0001570746,0.000042057694,0.0018354899],"genre_scores_gemma":[0.996798,0.00026909768,0.0016913965,0.00023096126,0.000030862604,0.0000048170255,0.00025276662,0.000013771014,0.0007083032],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998173,0.00003749815,0.00000799417,0.00006503167,0.00003530549,0.00003696689],"domain_scores_gemma":[0.9987225,0.0004482114,0.0001905218,0.0002856255,0.000181921,0.00017118768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001286885,0.0002789672,0.00038811308,0.0007402763,0.00050011603,0.0009287453,0.00052989396,0.00052129134,0.0012425226],"category_scores_gemma":[0.0017641027,0.000155585,0.00019496941,0.0006563963,0.0008710021,0.0010557149,0.00080683175,0.0004532959,0.00037212577],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003670935,0.00012497007,0.9204055,0.00011816615,0.00010641391,0.00045315037,0.0015725164,0.00112915,0.019735634,0.0056455913,0.0028906735,0.04745105],"study_design_scores_gemma":[0.00007047885,0.00021515659,0.96576756,0.00005077262,0.00010538296,0.0008132534,0.0014973348,0.005423652,0.004110461,0.010942776,0.010971972,0.000031122403],"about_ca_topic_score_codex":0.0028561484,"about_ca_topic_score_gemma":0.0038050727,"teacher_disagreement_score":0.0028561484,"about_ca_system_score_codex":0.00042786653,"about_ca_system_score_gemma":0.00021111302,"threshold_uncertainty_score":0.0068057775},"labels":[],"label_agreement":null},{"id":"W1971225616","doi":"10.1086/379066","title":"The Submillimeter Properties of Broad Absorption Line Quasars","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Astrophysics; Physics; Redshift; Galaxy; Sky; Astronomy; OVV quasar; Luminosity; Millimeter; Absorption (acoustics); Flux (metallurgy); Chemistry; Optics","score_opus":0.012668948644866585,"score_gpt":0.2089343872188744,"score_spread":0.1962654385740078,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971225616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99750805,0.00034512175,0.00051979854,0.000016274242,0.0000033905026,0.000009579751,0.0006279634,0.000029736731,0.000939962],"genre_scores_gemma":[0.9975078,0.00014809097,0.0006611704,0.000059808088,0.000011588026,0.000010941543,0.0010114243,0.0000107871765,0.00057836866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997843,0.000030431904,0.000014911912,0.00005603325,0.000052985226,0.00006135665],"domain_scores_gemma":[0.9988225,0.00015786229,0.0005463236,0.00014282111,0.00015385609,0.00017669186],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034873805,0.0003144784,0.00022868453,0.0014587999,0.00031352587,0.0005108485,0.00032428186,0.00016802964,0.0014620216],"category_scores_gemma":[0.0007619457,0.00020945488,0.0001711668,0.0009143322,0.00021158719,0.0003696124,0.0004674784,0.00029532067,0.000598511],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030673273,0.000041889387,0.9761307,0.000019759103,0.000039682734,0.00006901066,0.00029018548,0.00005786339,0.015101595,0.000055979242,0.00019343372,0.007969172],"study_design_scores_gemma":[0.0000010431376,0.0000467154,0.9982828,0.0000020607808,0.000008444545,0.00011482571,0.000059316197,0.00003674666,0.0007255063,0.00002045605,0.00069999666,0.000002225638],"about_ca_topic_score_codex":0.002448979,"about_ca_topic_score_gemma":0.0051573105,"teacher_disagreement_score":0.002448979,"about_ca_system_score_codex":0.00012985451,"about_ca_system_score_gemma":0.000101652025,"threshold_uncertainty_score":0.0048909187},"labels":[],"label_agreement":null},{"id":"W1971260591","doi":"10.1088/0004-637x/784/1/18","title":"THE STATE OF THE WARM AND COLD GAS IN THE EXTREME STARBURST AT THE CORE OF THE PHOENIX GALAXY CLUSTER (SPT-CLJ2344-4243)","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Goddard Space Flight Center; National Aeronautics and Space Administration; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Type-cD galaxy; Galaxy cluster; Intracluster medium; Brightest cluster galaxy; Nebula; Photoionization; Stars; Ionization","score_opus":0.009653629850486138,"score_gpt":0.20287819794766482,"score_spread":0.19322456809717867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971260591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963105,0.000017051834,0.00002554031,0.0000061426945,3.5961386e-7,0.0000011078504,0.000055843026,0.0000026887933,0.00026016703],"genre_scores_gemma":[0.99943393,0.00003166402,0.00012060796,0.000012424727,0.0000026544951,0.0000018377106,0.00022140844,0.0000021081353,0.00017335858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.0000030618837,0.0000016875272,0.000022211858,0.000008572054,0.000018278366],"domain_scores_gemma":[0.99989355,0.0000069619878,0.000038595674,0.0000067061674,0.000010700218,0.000043458473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012274362,0.00016223427,0.000121903904,0.00029262615,0.00026404392,0.00044676143,0.00027823646,0.00012711102,0.00083882146],"category_scores_gemma":[0.00019385813,0.00010134946,0.00008801743,0.00022228216,0.00023612905,0.00023582779,0.00053829,0.00020275466,0.00012587037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024501776,0.00008719597,0.9198689,0.00002311261,0.00006762644,0.00052302214,0.0006225132,0.0005685246,0.072135925,0.00020154496,0.00036965788,0.005286948],"study_design_scores_gemma":[0.0000068458967,0.00005147774,0.9971545,0.0000017569952,0.000009117644,0.00018077702,0.00013630679,0.0005155032,0.0015891752,0.000030075964,0.0003223074,0.0000022497097],"about_ca_topic_score_codex":0.011376534,"about_ca_topic_score_gemma":0.012658833,"teacher_disagreement_score":0.011376534,"about_ca_system_score_codex":0.00026422145,"about_ca_system_score_gemma":0.00012047226,"threshold_uncertainty_score":0.022620618},"labels":[],"label_agreement":null},{"id":"W1971297565","doi":"10.1088/0004-637x/777/2/121","title":"CORRELATING INFALL WITH DEUTERIUM FRACTIONATION IN DENSE CORES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; National Research Council Canada; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Deuterium; Astrophysics; Spectral line; Thermal; Signature (topology); Nuclear physics; Astronomy; Geometry; Thermodynamics","score_opus":0.007058382606632385,"score_gpt":0.2184244737110448,"score_spread":0.2113660911044124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971297565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996094,0.00009373227,0.00004493024,0.0000058258247,7.3834104e-7,0.0000014452294,0.00006922143,0.0000023415162,0.00017243078],"genre_scores_gemma":[0.99967265,0.000043650176,0.000075172866,0.000006662573,0.0000024290616,8.063009e-7,0.0001398049,0.0000011451892,0.000057656547],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983644,0.00001877748,0.000014261877,0.00004373263,0.000025724587,0.000061001716],"domain_scores_gemma":[0.998833,0.0001322315,0.00055886345,0.000059551527,0.00013926037,0.00027697743],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000289025,0.00020710242,0.00023422335,0.001260885,0.00034175575,0.0005140006,0.00019754202,0.00020514103,0.000680988],"category_scores_gemma":[0.0009146664,0.00016046317,0.00010927086,0.00078977755,0.0003072157,0.00028352605,0.00069186755,0.00014105218,0.00012113034],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000081887825,0.000011182383,0.9931257,0.000006461568,0.000014190357,0.00009930573,0.00008327411,0.000040596176,0.005047792,0.000017124936,0.000028857668,0.0014436096],"study_design_scores_gemma":[0.0000019823165,0.0000244373,0.998847,0.0000015498867,0.0000054198713,0.00014597198,0.0001040267,0.000085228865,0.0006333846,0.000015367194,0.00013411733,0.0000014753567],"about_ca_topic_score_codex":0.0066694617,"about_ca_topic_score_gemma":0.01217899,"teacher_disagreement_score":0.0066694617,"about_ca_system_score_codex":0.00026597784,"about_ca_system_score_gemma":0.00012533393,"threshold_uncertainty_score":0.013261259},"labels":[],"label_agreement":null},{"id":"W1971310733","doi":"10.1088/0004-637x/735/2/69","title":"STRUCTURE OF UNIFORMLY ROTATING STARS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Rotation (mathematics); Surface (topology); Physics; Constant (computer programming); Stars; Angular velocity; Geometry; Astrophysics; Mathematics; Classical mechanics","score_opus":0.013489342822784455,"score_gpt":0.21338834417603195,"score_spread":0.19989900135324748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971310733","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99514514,0.00017116309,0.002338535,0.000065943386,0.0000065730383,0.0000075582516,0.00010830965,0.000034989385,0.002121812],"genre_scores_gemma":[0.9986389,0.000052260068,0.00046945293,0.000016312966,0.0000053005624,0.000006519666,0.000264468,0.00001774815,0.00052888907],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998005,0.00004702686,0.000009380685,0.00005601439,0.000029108807,0.00005801557],"domain_scores_gemma":[0.9995189,0.000054984463,0.000099830024,0.00005678241,0.00011796283,0.00015157406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047251335,0.0004249954,0.000643927,0.00076767633,0.0006581593,0.0011371197,0.0014085391,0.00065114384,0.0014869261],"category_scores_gemma":[0.00171564,0.00044791173,0.00064591976,0.00041642698,0.0011787529,0.0007474939,0.0008590205,0.00057606405,0.0004765052],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006707864,0.000113236565,0.18621927,0.00008034563,0.00018687082,0.00064263656,0.00056167715,0.7352189,0.016490838,0.052646868,0.0011010779,0.0060673887],"study_design_scores_gemma":[0.00018177742,0.0003776493,0.07827889,0.000032791017,0.00006559833,0.00031473898,0.00025882563,0.89960194,0.0024254757,0.016736282,0.0016641801,0.00006174664],"about_ca_topic_score_codex":0.009984182,"about_ca_topic_score_gemma":0.004372696,"teacher_disagreement_score":0.009984182,"about_ca_system_score_codex":0.001995951,"about_ca_system_score_gemma":0.00068932475,"threshold_uncertainty_score":0.019852161},"labels":[],"label_agreement":null},{"id":"W1971365982","doi":"10.1088/0004-637x/702/1/805","title":"SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC): THE BOTTOM OF THE INITIAL MASS FUNCTION IN NGC 1333","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Cluster (spacecraft); Stars; Stellar mass; Low Mass; Spectroscopy; Stellar classification; Young stellar object","score_opus":0.00960518554972386,"score_gpt":0.23401378719956323,"score_spread":0.22440860164983936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971365982","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99890375,0.00006965148,0.00012785885,0.000011002446,0.0000018153456,0.000004582235,0.00035557084,0.000024295103,0.0005014963],"genre_scores_gemma":[0.99731725,0.00005521223,0.0004577266,0.0000125926035,0.000003146617,0.000007869143,0.0017112643,0.000008593225,0.00042638392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998989,0.000007972599,0.0000074040295,0.000024483808,0.00002901281,0.00003227828],"domain_scores_gemma":[0.99955803,0.00003815832,0.00012549094,0.00003339101,0.00008784799,0.00015714037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021542398,0.00014453083,0.0002272114,0.00084805733,0.00061170955,0.0004432056,0.00019043022,0.00013441886,0.0013484604],"category_scores_gemma":[0.00042092835,0.00008470904,0.00015477164,0.001128911,0.00025358805,0.0002208686,0.000636197,0.00018598905,0.00030774015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013212259,0.000027141703,0.97573406,0.000022106742,0.000014662335,0.0003139104,0.0006499457,0.00022172586,0.011704307,0.00017919231,0.00074509816,0.01025559],"study_design_scores_gemma":[0.0000018946073,0.000018469516,0.9983272,0.0000026379835,0.0000041075928,0.00015384889,0.00013891602,0.00018828902,0.00046114912,0.00001972683,0.0006811626,0.0000026291953],"about_ca_topic_score_codex":0.04041706,"about_ca_topic_score_gemma":0.060277287,"teacher_disagreement_score":0.04041706,"about_ca_system_score_codex":0.0005416346,"about_ca_system_score_gemma":0.00042503956,"threshold_uncertainty_score":0.08036363},"labels":[],"label_agreement":null},{"id":"W1971418912","doi":"10.1088/0004-637x/710/1/783","title":"THE LOCAL ENVIRONMENTS OF INTERACTING GALAXY SYSTEMS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Quasar; Active galactic nucleus; Peculiar galaxy; Universe; Astronomy; Luminosity; Luminosity function; Galaxy formation and evolution; Galaxy group","score_opus":0.00495600792673358,"score_gpt":0.20290987323038012,"score_spread":0.19795386530364653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971418912","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907625,0.000111056994,0.0002225825,0.000005265832,3.0620438e-7,0.0000018383865,0.00005578649,0.00000541663,0.0005214331],"genre_scores_gemma":[0.9996712,0.000045503573,0.0001260567,0.0000017596415,0.0000013145979,0.0000013154607,0.0000845223,0.0000015090636,0.00006688127],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997216,0.00006390191,0.00001961709,0.000091254085,0.000043169388,0.000060492577],"domain_scores_gemma":[0.99885535,0.00022993516,0.00047029904,0.00012331015,0.00011398018,0.00020714433],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018338459,0.0001257979,0.00031899766,0.0012157619,0.0003923893,0.00080323394,0.00023378848,0.00014241053,0.0014962116],"category_scores_gemma":[0.0014562343,0.00012444577,0.0001110934,0.000902967,0.0005933645,0.0004969536,0.0010285175,0.000119222816,0.00027293936],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022435946,0.000029686918,0.967878,0.000060826413,0.00010186585,0.00036001462,0.0017013219,0.0013084557,0.018735355,0.00097059814,0.000104816754,0.00852485],"study_design_scores_gemma":[0.0000034462341,0.000051231862,0.99651057,0.0000038321828,0.000027240063,0.0003993345,0.00079144613,0.00062421756,0.00077165756,0.00041891544,0.00038927433,0.000008899707],"about_ca_topic_score_codex":0.0016287349,"about_ca_topic_score_gemma":0.002840136,"teacher_disagreement_score":0.0016287349,"about_ca_system_score_codex":0.00022259011,"about_ca_system_score_gemma":0.00010309888,"threshold_uncertainty_score":0.0050053596},"labels":[],"label_agreement":null},{"id":"W1971446808","doi":"10.1088/0004-637x/701/2/1534","title":"PHOTOMETRIC VARIABILITY OF THE T2.5 BROWN DWARF SIMP J013656.5+093347: EVIDENCE FOR EVOLVING WEATHER PATTERNS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":268,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Université de Montréal; Centre for Research in Astrophysics of Québec; Université du Québec à Montréal","funders":"","keywords":"Brown dwarf; Photometry (optics); Light curve; Amplitude; Astrophysics; Physics; Rotation period; Dwarf planet; Astronomy; Planet; Optics; Stars","score_opus":0.02412503213891019,"score_gpt":0.26818544875990885,"score_spread":0.24406041662099867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971446808","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995326,0.000035486093,0.00006884718,0.000009644542,0.000001258312,0.0000012281754,0.00010647082,0.00000962331,0.0002348329],"genre_scores_gemma":[0.9995819,0.000015628915,0.00009698409,0.000007351839,0.0000029561375,0.0000011654106,0.00022972525,0.000002356211,0.00006194067],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993455,0.0000054285156,0.0000048266565,0.00002018551,0.000019735313,0.000015293364],"domain_scores_gemma":[0.99978334,0.000012945751,0.00008457727,0.000020337178,0.00002676736,0.000071960465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013049066,0.00016490718,0.00020680249,0.00054745865,0.00028927834,0.00029001952,0.00017669713,0.00018429785,0.0005664223],"category_scores_gemma":[0.00027104243,0.00010927722,0.00013760476,0.0005724852,0.00029829043,0.00017871142,0.00032789548,0.00016032584,0.00018094388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002719561,0.00004718917,0.8333012,0.000046925023,0.0000397569,0.000738469,0.00048562558,0.0003048853,0.15691215,0.00022240524,0.00039365827,0.007235738],"study_design_scores_gemma":[0.000003866598,0.00004510996,0.99734217,0.0000024703243,0.000008325005,0.00032029435,0.000091029775,0.0003225329,0.0014861919,0.000040952382,0.00033314523,0.00000387083],"about_ca_topic_score_codex":0.004562106,"about_ca_topic_score_gemma":0.007868003,"teacher_disagreement_score":0.004562106,"about_ca_system_score_codex":0.00032749935,"about_ca_system_score_gemma":0.00011622516,"threshold_uncertainty_score":0.009071112},"labels":[],"label_agreement":null},{"id":"W1971481635","doi":"10.1086/589633","title":"Number Density Evolution of<i>K</i><sub><i>s</i></sub>‐Band–Selected High‐Redshift Galaxy Populations in the<i>AKARI</i>North Ecliptic Pole Field","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Galaxy; Redshift; Source counts; Population; Luminosity; Number density; Hubble Deep Field","score_opus":0.00984418591517198,"score_gpt":0.21001439109582984,"score_spread":0.20017020518065787,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971481635","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986915,0.000028171531,0.00013012266,0.00001554937,9.686804e-7,0.0000020363025,0.00042066126,0.000015131599,0.00069597224],"genre_scores_gemma":[0.99858725,0.000018075463,0.00013374312,0.0000043900295,0.0000023927025,0.0000029947144,0.0008420241,0.0000025936374,0.00040657618],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999884,0.000018927281,0.000007354096,0.000038847444,0.000025265259,0.000025554253],"domain_scores_gemma":[0.9987925,0.0002775368,0.0004814434,0.00009287536,0.00021723783,0.00013821716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023787624,0.00011676013,0.00010741613,0.0010228592,0.0001523924,0.0003816534,0.000313539,0.00026128697,0.0028365043],"category_scores_gemma":[0.0010217972,0.00013887402,0.00015478196,0.00052610936,0.00027519462,0.00035728983,0.00020908315,0.0001357901,0.0005118928],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000076418335,0.000019493396,0.98730904,0.0000099621975,0.000024527264,0.00006357036,0.00013211086,0.004098132,0.0025631615,0.0004329551,0.0005579833,0.0047127595],"study_design_scores_gemma":[0.0000021558035,0.000015730413,0.99495935,0.0000015949548,0.00000561672,0.000061061524,0.000054518012,0.004273149,0.00033442065,0.0000686045,0.00022062557,0.0000031630684],"about_ca_topic_score_codex":0.011433403,"about_ca_topic_score_gemma":0.009544139,"teacher_disagreement_score":0.011433403,"about_ca_system_score_codex":0.00067555916,"about_ca_system_score_gemma":0.00010313329,"threshold_uncertainty_score":0.022733688},"labels":[],"label_agreement":null},{"id":"W1971511089","doi":"10.1088/0004-637x/777/2/85","title":"DEUTERATED MOLECULES IN ORION KL FROM<i>HERSCHEL</i>/HIFI","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of New Brunswick","funders":"","keywords":"Isotopologue; Deuterium; Astrochemistry; Molecular cloud; Interstellar medium; Molecule; Hydrogen molecule; Abundance (ecology); Cosmochemistry","score_opus":0.008079292801089448,"score_gpt":0.21927480772602206,"score_spread":0.2111955149249326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971511089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98553616,0.0012194277,0.00043351634,0.000067950794,0.000009015915,0.000009528354,0.008007619,0.00017981806,0.0045369235],"genre_scores_gemma":[0.9702545,0.0009094356,0.0030253974,0.00017159953,0.000033532884,0.000018147137,0.023232888,0.0001636384,0.002190952],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998406,0.000004726081,0.0000041099493,0.000052897933,0.000057589627,0.000040134924],"domain_scores_gemma":[0.9998374,0.000012513857,0.0000723257,0.000019040854,0.000029319483,0.000029307657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013434979,0.0004110558,0.00024616314,0.0016350852,0.00041283155,0.0005144542,0.0003801086,0.0002789696,0.0014194037],"category_scores_gemma":[0.00016508183,0.0001653203,0.00018445626,0.0016417408,0.00020420509,0.00042468437,0.00059309986,0.000184213,0.0004903348],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006678714,0.000110084606,0.500226,0.00040846976,0.00029369153,0.001247864,0.0013054134,0.0021786145,0.42274055,0.00047873307,0.005804778,0.06453789],"study_design_scores_gemma":[0.000016644291,0.000062689105,0.9433737,0.000024618264,0.00007270274,0.00060448295,0.00025467103,0.001446368,0.026845599,0.00011964271,0.027142761,0.000036191475],"about_ca_topic_score_codex":0.020183386,"about_ca_topic_score_gemma":0.031669665,"teacher_disagreement_score":0.020183386,"about_ca_system_score_codex":0.00076322426,"about_ca_system_score_gemma":0.00022166799,"threshold_uncertainty_score":0.040131807},"labels":[],"label_agreement":null},{"id":"W1971535979","doi":"10.1088/0004-637x/747/2/89","title":"THE DOUBLE PULSAR ECLIPSES. I. PHENOMENOLOGY AND MULTI-FREQUENCY ANALYSIS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University; Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Fonds Québécois de la Recherche sur la Nature et les Technologies; Killam Trusts; Canada Research Chairs; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Pulsar; Magnetosphere; Millisecond pulsar; Binary pulsar; X-ray pulsar; Magnetar; Phenomenology (philosophy); Plasma; Neutron star","score_opus":0.0219456855501419,"score_gpt":0.3336795019820879,"score_spread":0.311733816431946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971535979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9762491,0.0037918822,0.011018002,0.000198176,0.000030434372,0.000038945687,0.00019364915,0.00004486787,0.008434835],"genre_scores_gemma":[0.99699116,0.00048007644,0.0019191406,0.00002267661,0.000030706953,0.000014526725,0.000101022866,0.00000807714,0.00043265946],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.000016740625,0.000005385765,0.00001941624,0.00002244135,0.000019037903],"domain_scores_gemma":[0.9994431,0.00019957533,0.00017557941,0.00008237752,0.000043172022,0.000056224402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024208598,0.0001865695,0.00018943379,0.0009653686,0.0003167484,0.00060926,0.00023397626,0.00022754638,0.0007649977],"category_scores_gemma":[0.00078112894,0.0001406093,0.000296177,0.0004663408,0.0006093906,0.0006700905,0.0006119842,0.00041679616,0.00007269257],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015171568,0.00040085596,0.43179142,0.00087883254,0.00030196793,0.0068976404,0.0031381494,0.021366427,0.18633394,0.14785503,0.003264661,0.19625397],"study_design_scores_gemma":[0.00007424822,0.00055637065,0.78751904,0.00013287044,0.00011623622,0.011706792,0.0016347374,0.08290413,0.010281434,0.08410061,0.020870607,0.00010290155],"about_ca_topic_score_codex":0.00053033384,"about_ca_topic_score_gemma":0.00063677446,"teacher_disagreement_score":0.0009653686,"about_ca_system_score_codex":0.00029696332,"about_ca_system_score_gemma":0.00011630809,"threshold_uncertainty_score":0.002559185},"labels":[],"label_agreement":null},{"id":"W1971543949","doi":"10.1086/346261","title":"Neutral Beams from Blazar Jets","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":243,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Lorentz factor; Neutron; Photon; Blazar; Radiation; Nuclear physics; Neutrino; Gamma ray; Astrophysics; Atomic physics; Optics; Lorentz transformation","score_opus":0.008081126857271439,"score_gpt":0.21085142888350492,"score_spread":0.20277030202623347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971543949","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.31310102,0.010321167,0.32220784,0.0041641057,0.0015907872,0.00062410854,0.00096629484,0.0008772306,0.34614754],"genre_scores_gemma":[0.8957184,0.004273865,0.01993009,0.0018607066,0.0010688916,0.0006161564,0.00061147107,0.00021567641,0.07570486],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997429,0.00007374165,0.0000072604307,0.000025915147,0.000092752714,0.000057412693],"domain_scores_gemma":[0.99982625,0.00003316161,0.000058817728,0.000014752836,0.000028006618,0.000039059767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000530898,0.0014116076,0.00071683025,0.00045690202,0.0010793915,0.0018616688,0.0014898678,0.0022237527,0.0065495735],"category_scores_gemma":[0.00078241475,0.00056049944,0.0010475308,0.000718387,0.0012917031,0.0015023234,0.0016075049,0.0012457115,0.00087477645],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025785767,0.00014175038,0.0036202634,0.0002675465,0.00009594531,0.0013849335,0.00046648705,0.19737487,0.011090833,0.7711387,0.004759995,0.009400746],"study_design_scores_gemma":[0.0007432548,0.00050912634,0.005203648,0.00018925351,0.00007938089,0.0010994727,0.0004913579,0.64554566,0.003135627,0.30828002,0.034589585,0.00013356574],"about_ca_topic_score_codex":0.005759302,"about_ca_topic_score_gemma":0.0036075483,"teacher_disagreement_score":0.0065495735,"about_ca_system_score_codex":0.0017236547,"about_ca_system_score_gemma":0.0007386974,"threshold_uncertainty_score":0.021910489},"labels":[],"label_agreement":null},{"id":"W1971856568","doi":"10.1086/379093","title":"A Second Glitch from the \"Anomalous\" X-Ray Pulsar 1RXS J170849.0-4000910","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Glitch; Pulsar; Astrophysics; Physics; Astronomy; Optics","score_opus":0.010331340345751512,"score_gpt":0.2816863057684053,"score_spread":0.2713549654226538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971856568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981173,0.00015557166,0.000688002,0.000047773632,0.000027637845,0.000016104937,0.00022064302,0.000055174853,0.0006718171],"genre_scores_gemma":[0.995752,0.00012487416,0.0014889608,0.0001301604,0.000047611582,0.000027155595,0.001581204,0.000026029053,0.0008220497],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998816,0.0000068963664,0.000006481379,0.000030217438,0.00004582211,0.000028981669],"domain_scores_gemma":[0.99948525,0.000059473798,0.0002410571,0.00006388791,0.00004871998,0.0001015828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020568787,0.00037640566,0.00038705269,0.00051705213,0.00047268675,0.0003394825,0.00028824594,0.0005801149,0.0005484544],"category_scores_gemma":[0.00043864772,0.00017336602,0.00036948288,0.0003532456,0.00023605903,0.00020830451,0.00086120836,0.0010245675,0.00022186631],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011905432,0.00038827097,0.23824012,0.00024987815,0.00028366092,0.010452903,0.0010490192,0.0010295141,0.7080726,0.00061838835,0.0018346754,0.036590375],"study_design_scores_gemma":[0.000048925856,0.0014101355,0.9390045,0.000022047081,0.00008762939,0.007783528,0.00015324856,0.0017314206,0.044474516,0.00019201504,0.005036929,0.00005516143],"about_ca_topic_score_codex":0.0010218302,"about_ca_topic_score_gemma":0.0021231289,"teacher_disagreement_score":0.0010218302,"about_ca_system_score_codex":0.00015075027,"about_ca_system_score_gemma":0.00012854271,"threshold_uncertainty_score":0.002031684},"labels":[],"label_agreement":null},{"id":"W1971909548","doi":"10.1086/324297","title":"Statistical Properties of Galactic Starlight Polarization","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Starlight; Physics; Galactic plane; Astrophysics; Polarization (electrochemistry); Linear polarization; Polarization in astronomy; Astronomy; Degree of polarization; Milky Way; Sky; Multipole expansion; Interstellar medium; Stars; Magnetic field; Circular polarization; Galaxy; Optics; Scattering","score_opus":0.016315505020223994,"score_gpt":0.21750798872558721,"score_spread":0.20119248370536322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971909548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931378,0.00014924408,0.002952902,0.000049192997,0.0000057498264,0.000006374081,0.0026235029,0.00010381445,0.0009714249],"genre_scores_gemma":[0.99547535,0.00005940615,0.00037785867,0.000006529958,0.000015954405,0.000005991295,0.003955545,0.000020108911,0.000083318606],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992661,0.00017323939,0.00004622698,0.00022856152,0.0001727173,0.000113168826],"domain_scores_gemma":[0.9879693,0.007436755,0.0018643609,0.0012222457,0.0010523644,0.00045508423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011823401,0.00018975469,0.0002644836,0.0025095053,0.0002580785,0.0010471176,0.00024709996,0.00019928114,0.0009865382],"category_scores_gemma":[0.007878652,0.00009742354,0.00037166683,0.0021842604,0.00052656693,0.0003987487,0.00044303617,0.00032787363,0.0003210531],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014849727,0.000029719824,0.9686875,0.000027026243,0.00016470463,0.0001519314,0.00011311285,0.0090079615,0.003884326,0.0010328713,0.00086985197,0.015882343],"study_design_scores_gemma":[0.0000054950656,0.0000648586,0.9615934,0.0000064121464,0.000035912035,0.0003542931,0.00014891742,0.033777744,0.0018234472,0.00092897186,0.0012367347,0.000023823719],"about_ca_topic_score_codex":0.0021222753,"about_ca_topic_score_gemma":0.0010670715,"teacher_disagreement_score":0.0025095053,"about_ca_system_score_codex":0.00024524363,"about_ca_system_score_gemma":0.00020561632,"threshold_uncertainty_score":0.0062528253},"labels":[],"label_agreement":null},{"id":"W1971918524","doi":"10.1086/318368","title":"<i>Ginga</i>Observations of Hercules X‐1: Spectrum Dependence on 35 Day Phase","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Spectral line; Astrophysics; Equivalent width; Accretion disc; Emission spectrum; Atomic physics; Astronomy","score_opus":0.026462323275442286,"score_gpt":0.26566724512027756,"score_spread":0.23920492184483527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971918524","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99055016,0.00021098746,0.00038885552,0.00007755033,0.000006027407,0.000014943434,0.0056816167,0.00032275156,0.0027470207],"genre_scores_gemma":[0.9866549,0.00012311678,0.00081181095,0.000057308098,0.000018331168,0.000016317612,0.01137664,0.00008025578,0.00086127094],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998957,0.000011648247,0.000006216772,0.000033581793,0.000026618083,0.00002627287],"domain_scores_gemma":[0.99938726,0.00009725842,0.000239385,0.000100169804,0.00008449943,0.000091507274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026453505,0.00041646432,0.00023385517,0.0011440292,0.00024116378,0.00040551403,0.00028264025,0.00025449926,0.0016358186],"category_scores_gemma":[0.00044843613,0.00020479629,0.00018921519,0.00096325873,0.00017714163,0.00025125072,0.00031341112,0.0002834893,0.0006133067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001313924,0.0001714982,0.8624493,0.00018883613,0.00029253482,0.00081452704,0.00041730038,0.003718658,0.0939968,0.00045939218,0.008718251,0.027458947],"study_design_scores_gemma":[0.000008626873,0.00003394407,0.9960168,0.0000031461243,0.000009882782,0.00012103067,0.000012090844,0.0005740298,0.0016793336,0.00003748594,0.0014980269,0.0000055537926],"about_ca_topic_score_codex":0.005089556,"about_ca_topic_score_gemma":0.01070575,"teacher_disagreement_score":0.005089556,"about_ca_system_score_codex":0.00034974137,"about_ca_system_score_gemma":0.00007808124,"threshold_uncertainty_score":0.010119855},"labels":[],"label_agreement":null},{"id":"W1971966109","doi":"10.1088/0004-637x/708/1/698","title":"THE ACS SURVEY OF GALACTIC GLOBULAR CLUSTERS. IX. HORIZONTAL BRANCH MORPHOLOGY AND THE SECOND PARAMETER PHENOMENON","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":455,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Globular cluster; Horizontal branch; Morphology (biology); Metallicity; Stellar evolution; Computational astrophysics; Stellar dynamics","score_opus":0.010998810617902336,"score_gpt":0.2251445890711843,"score_spread":0.21414577845328195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1971966109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.55039424,0.0102430675,0.0018383217,0.0037214726,0.00042038865,0.00015892166,0.32889676,0.00071849,0.10360834],"genre_scores_gemma":[0.7668721,0.0058179363,0.004057041,0.0007134497,0.00044299057,0.00011638208,0.19361646,0.00011638308,0.028247233],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998313,0.0000129591945,0.000013996031,0.000026771964,0.00008174848,0.000033258537],"domain_scores_gemma":[0.9994223,0.000034548295,0.000113963775,0.000059533835,0.00024323937,0.00012627277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029483173,0.00024136485,0.00019129792,0.0030254666,0.00026025466,0.0006860537,0.0002934148,0.0002105395,0.0039538895],"category_scores_gemma":[0.00075590255,0.000098298384,0.00014263381,0.0050289147,0.00013802541,0.00042909535,0.0005525058,0.000204457,0.002310761],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012055307,0.00005003173,0.7182419,0.00023453773,0.00009019119,0.00012803945,0.00020509762,0.00030535244,0.0024381555,0.004749405,0.18824495,0.08519197],"study_design_scores_gemma":[0.000008838225,0.000009992544,0.94144595,0.000026294003,0.000012273821,0.000057171317,0.0001434433,0.00013328907,0.00025817085,0.000452526,0.057448324,0.0000037048126],"about_ca_topic_score_codex":0.045789167,"about_ca_topic_score_gemma":0.062924944,"teacher_disagreement_score":0.045789167,"about_ca_system_score_codex":0.0006280519,"about_ca_system_score_gemma":0.000552614,"threshold_uncertainty_score":0.09104532},"labels":[],"label_agreement":null},{"id":"W1972203853","doi":"10.1086/344815","title":"STACEE Observations of Markarian 421 during an Extended Gamma-Ray Outburst","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; TRIUMF; McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Gamma ray; Flux (metallurgy); Light curve; Astronomy","score_opus":0.02080280619430955,"score_gpt":0.22148981012457641,"score_spread":0.20068700393026687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972203853","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99656665,0.000052348947,0.000118952026,0.000030430218,0.0000024643223,0.0000034138307,0.0003780756,0.000032613345,0.0028149472],"genre_scores_gemma":[0.9968219,0.000083195,0.00040527608,0.00003679868,0.000006463789,0.0000054352126,0.0012715933,0.000016734355,0.0013528077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988484,0.0000075077646,0.000003910479,0.000025661582,0.00004356565,0.000034583703],"domain_scores_gemma":[0.9996965,0.000025625839,0.00006247658,0.000047257,0.00007473767,0.000093525865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018505398,0.0001575513,0.0003075407,0.00091999234,0.0007531278,0.0005742131,0.0003124412,0.00034558366,0.00075656944],"category_scores_gemma":[0.00041134589,0.0002752206,0.0001600045,0.00076133816,0.00019912084,0.0002432825,0.0007644894,0.0003310794,0.00039375984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001392346,0.00027453233,0.71786386,0.00009255456,0.0002096732,0.0022114352,0.0030995703,0.0008334595,0.24544734,0.001159038,0.0030427936,0.024373405],"study_design_scores_gemma":[0.000014516556,0.00007423045,0.98977953,0.000004648779,0.00001876129,0.00044913683,0.00018868528,0.0003255057,0.0056927134,0.00004588324,0.003396154,0.000010246414],"about_ca_topic_score_codex":0.006706954,"about_ca_topic_score_gemma":0.025627743,"teacher_disagreement_score":0.006706954,"about_ca_system_score_codex":0.00030919086,"about_ca_system_score_gemma":0.00015275566,"threshold_uncertainty_score":0.013335824},"labels":[],"label_agreement":null},{"id":"W1972218288","doi":"10.1088/0004-637x/709/2/937","title":"REDSHIFT EVOLUTION IN BLACK HOLE-BULGE RELATIONS: TESTING C IV-BASED BLACK HOLE MASSES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Balmer series; Astrophysics; Physics; Redshift; Bulge; Quasar; Galaxy; Black hole (networking); Spectroscopy; Astronomy; Spectral line; Emission spectrum","score_opus":0.010905572830269997,"score_gpt":0.22438972091419526,"score_spread":0.21348414808392527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972218288","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99894613,0.000057850182,0.00024837634,0.000029550476,0.0000023359048,0.0000033467627,0.00007945204,0.000007690059,0.0006251304],"genre_scores_gemma":[0.99980444,0.000007698597,0.00007329269,0.000005034098,0.0000024069477,0.0000011132846,0.00005425711,0.0000020939804,0.000049736063],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993793,0.00022325727,0.000046527904,0.0001393408,0.00012441128,0.000087078406],"domain_scores_gemma":[0.9805577,0.008182667,0.006769122,0.0023713158,0.0010840205,0.0010351858],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022400792,0.00038081984,0.00018298234,0.0017783357,0.00040370025,0.0009978281,0.0006931604,0.00043989933,0.002129374],"category_scores_gemma":[0.015910571,0.00012218437,0.00029632077,0.0007046027,0.0010942244,0.0011025675,0.00089198473,0.0005226503,0.00028156175],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014645843,0.00003070688,0.99529797,0.000003879953,0.000050395287,0.000038081667,0.0002971705,0.0003101732,0.0010709658,0.0003060758,0.00003849879,0.002409728],"study_design_scores_gemma":[0.000005790605,0.00009684541,0.9965869,0.0000029754908,0.000024693307,0.000057565856,0.00025826306,0.0016442294,0.0008222962,0.00036477516,0.00013115485,0.0000045344304],"about_ca_topic_score_codex":0.00795246,"about_ca_topic_score_gemma":0.003619678,"teacher_disagreement_score":0.00795246,"about_ca_system_score_codex":0.0005279832,"about_ca_system_score_gemma":0.0001700664,"threshold_uncertainty_score":0.015812337},"labels":[],"label_agreement":null},{"id":"W1972280282","doi":"10.1088/0004-637x/736/2/94","title":"THE GRADIENTS IN THE 47 Tuc RED GIANT BRANCH BUMP AND HORIZONTAL BRANCH ARE CONSISTENT WITH A CENTRALLY CONCENTRATED, HELIUM-ENRICHED SECOND STELLAR GENERATION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Red-giant branch; Horizontal branch; Stars; Giant star; Red giant; Photometry (optics); Asymptotic giant branch; Helium","score_opus":0.016011283687039263,"score_gpt":0.19743561261950945,"score_spread":0.18142432893247018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972280282","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977773,0.00005463812,0.00018676322,0.000021155367,0.000004193909,0.000004008013,0.00009680033,0.00003313701,0.0018219987],"genre_scores_gemma":[0.99921787,0.000020443935,0.00023232994,0.000012973186,0.0000057049556,0.0000032001442,0.00017417643,0.0000061336473,0.00032711757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998629,0.000004558682,0.0000041670046,0.000038858554,0.000040579198,0.000048975315],"domain_scores_gemma":[0.9992957,0.00005106843,0.0002821726,0.000070840724,0.000097450786,0.0002027486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015035363,0.00031023522,0.0003629643,0.001172742,0.00065564475,0.0007969304,0.00041809285,0.00041610518,0.0025057883],"category_scores_gemma":[0.0004057424,0.00017379236,0.00020841102,0.00062756566,0.00048258607,0.00021416631,0.00045978074,0.00030037283,0.0004808889],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026189585,0.000040517116,0.8703781,0.000036781716,0.00005533229,0.00040119578,0.00041011415,0.00036234563,0.12116595,0.00085949275,0.0004770567,0.005551202],"study_design_scores_gemma":[0.0000044340463,0.00003334061,0.99525887,0.0000031700367,0.000010698529,0.00022799562,0.00010100798,0.00042451592,0.00352811,0.00011635875,0.00028744712,0.0000040749055],"about_ca_topic_score_codex":0.0047999187,"about_ca_topic_score_gemma":0.0104612,"teacher_disagreement_score":0.0047999187,"about_ca_system_score_codex":0.0004233699,"about_ca_system_score_gemma":0.00023443962,"threshold_uncertainty_score":0.009544015},"labels":[],"label_agreement":null},{"id":"W1972308849","doi":"10.1086/521820","title":"Multiwavelength Study of Massive Galaxies at<i>z</i> ∼ 2. II. Widespread Compton‐thick Active Galactic Nuclei and the Concurrent Growth of Black Holes and Bulges","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":346,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Star formation; Redshift; Luminous infrared galaxy; Luminosity; Astronomy; Population; Extragalactic astronomy","score_opus":0.008765323088336809,"score_gpt":0.22730794638341575,"score_spread":0.21854262329507895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972308849","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990281,0.00014057709,0.00007056274,0.00003084484,0.0000015159718,0.0000032750831,0.00016337006,0.00001131743,0.0005504941],"genre_scores_gemma":[0.999025,0.00008213734,0.00022526665,0.000023329154,0.000010190994,0.000003805308,0.00029913077,0.0000034716193,0.00032765509],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999043,0.0000060769494,0.0000045859238,0.000026425678,0.000015758378,0.000042918928],"domain_scores_gemma":[0.99960583,0.000024714076,0.00015694571,0.000024509662,0.000032243654,0.00015571516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014627373,0.0002341211,0.00018799397,0.0015920443,0.00034155333,0.0006002706,0.00026406557,0.00022904591,0.0007717329],"category_scores_gemma":[0.00023071209,0.00020008023,0.00023662375,0.0007676807,0.0001907184,0.00027986016,0.00044627328,0.00031527216,0.0003341661],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011997474,0.00005303996,0.9572623,0.000017318436,0.00003977123,0.00045459412,0.00047958552,0.000065412336,0.03342279,0.0001967667,0.00023001968,0.0076584294],"study_design_scores_gemma":[8.130769e-7,0.000015228098,0.99938595,0.0000010348126,0.00000344362,0.00017231514,0.000060884806,0.000029023406,0.0001908978,0.000012304073,0.00012727806,8.7832285e-7],"about_ca_topic_score_codex":0.004368988,"about_ca_topic_score_gemma":0.008649213,"teacher_disagreement_score":0.004368988,"about_ca_system_score_codex":0.00030429053,"about_ca_system_score_gemma":0.0000851834,"threshold_uncertainty_score":0.008687139},"labels":[],"label_agreement":null},{"id":"W1972315382","doi":"10.1086/320244","title":"Space Telescope Imaging Spectrograph Echelle Observations of the Seyfert Galaxy NGC 4151: Physical Conditions in the Ultraviolet Absorbers","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Space Telescope Imaging Spectrograph; Physics; Astrophysics; Galaxy; Spectrograph; Ionization; Emission spectrum; Spectral line; Astronomy; Absorption (acoustics); Absorption spectroscopy; Hubble space telescope; Optics; Ion","score_opus":0.009893891789117067,"score_gpt":0.22813936147427982,"score_spread":0.21824546968516276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972315382","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994703,0.000011909518,0.00010181706,0.00000713891,4.3646082e-7,0.0000015630368,0.00017326488,0.000017553019,0.00021596997],"genre_scores_gemma":[0.99884254,0.000015168334,0.00034920007,0.0000039585684,0.000001485133,0.000002080978,0.0006479029,0.0000044149615,0.00013333828],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999058,0.000016778733,0.000005441276,0.000026143169,0.000021541444,0.000024208288],"domain_scores_gemma":[0.999676,0.000054866174,0.000109911496,0.00004849927,0.000037679027,0.000073108415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033383846,0.00024542797,0.00016234646,0.000685061,0.00042428335,0.0003843529,0.00026694423,0.00024726163,0.0010343397],"category_scores_gemma":[0.0005279719,0.00015206738,0.00025597983,0.000561801,0.00015897222,0.00037011606,0.00027390258,0.0002209379,0.0001830153],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017008213,0.00008716705,0.9599796,0.000026020876,0.00007802523,0.00030596452,0.0005427917,0.011140354,0.020868598,0.0002256878,0.00025996182,0.006315661],"study_design_scores_gemma":[0.000008841919,0.000055344753,0.9906889,0.0000032178093,0.000020284533,0.00007563194,0.00010837486,0.0067787827,0.0018456003,0.00006367633,0.00034438798,0.0000069436705],"about_ca_topic_score_codex":0.01528765,"about_ca_topic_score_gemma":0.0265301,"teacher_disagreement_score":0.01528765,"about_ca_system_score_codex":0.00055642234,"about_ca_system_score_gemma":0.0001337243,"threshold_uncertainty_score":0.030397296},"labels":[],"label_agreement":null},{"id":"W1972315967","doi":"10.1088/0004-637x/690/1/773","title":"<i>XMM-NEWTON</i>VIEW OF THE MULTIPHASE WARM ABSORBER IN SEYFERT 1 GALAXY NGC 985","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Ionization; Physics; Absorption (acoustics); EPIC; Astrophysics; Galaxy; Spectral line; Absorption spectroscopy; Atomic physics; Ion; Optics; Astronomy","score_opus":0.017405161797033053,"score_gpt":0.2353519986364689,"score_spread":0.21794683683943586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972315967","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98350865,0.0010510755,0.0014171229,0.00030844298,0.000021972894,0.000020416885,0.0017664457,0.0002530489,0.011652867],"genre_scores_gemma":[0.99294937,0.00031875045,0.0026293127,0.00013066942,0.0000930302,0.000012265653,0.0013783053,0.000028969753,0.0024593314],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999573,0.0000030333476,0.0000023572693,0.00001282873,0.000014237563,0.000010250199],"domain_scores_gemma":[0.9998586,0.000014488753,0.000064550484,0.000011728762,0.000016712005,0.000033822107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009170608,0.00032021003,0.0001316835,0.0024392921,0.00034212266,0.00049783755,0.00028236097,0.00046158125,0.0026745447],"category_scores_gemma":[0.0001304134,0.00012767673,0.00039444942,0.000629719,0.00013423903,0.00024505876,0.0002309641,0.00025614488,0.00051730033],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005989816,0.00028215258,0.7300808,0.00018587394,0.0002867558,0.0056414325,0.0006493791,0.00852097,0.19314022,0.0025846865,0.007961842,0.050066974],"study_design_scores_gemma":[0.0000054756833,0.000033877903,0.99133354,0.000014725555,0.00003024861,0.00036333848,0.000053866614,0.004503395,0.0012308127,0.00016677912,0.002258725,0.0000052860996],"about_ca_topic_score_codex":0.005899637,"about_ca_topic_score_gemma":0.007444035,"teacher_disagreement_score":0.005899637,"about_ca_system_score_codex":0.00044743996,"about_ca_system_score_gemma":0.000065546155,"threshold_uncertainty_score":0.011730611},"labels":[],"label_agreement":null},{"id":"W1972347701","doi":"10.1088/0004-637x/703/1/198","title":"DYNAMICS OF LYMAN BREAK GALAXIES AND THEIR HOST HALOS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Redshift; Halo; Galaxy formation and evolution; Knot (papermaking); Dark matter; Stellar mass","score_opus":0.004608215445312815,"score_gpt":0.1945694792533683,"score_spread":0.18996126380805547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972347701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993318,0.000092603485,0.00007408081,0.00001002028,4.885518e-7,0.0000017991792,0.000074572024,0.0000073717747,0.00040729664],"genre_scores_gemma":[0.99957174,0.000033513523,0.00007079241,0.000004344579,0.000001948488,0.0000013999371,0.00014880426,0.0000021368162,0.00016539349],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982625,0.00002086675,0.000006879746,0.00003269472,0.0000343944,0.00007882566],"domain_scores_gemma":[0.9988174,0.0001341333,0.00044575374,0.000053187352,0.00009214321,0.00045732388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000344099,0.00022138028,0.00017274212,0.0022445952,0.00031550365,0.0010229197,0.00028552176,0.0002330294,0.0018856075],"category_scores_gemma":[0.0011658814,0.0001744169,0.00017449558,0.00061524165,0.00039890496,0.00050946843,0.0008961773,0.0002246735,0.00030450875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001365972,0.000024147519,0.99006444,0.000007193716,0.000033603676,0.00009704805,0.000385339,0.00043604392,0.005392376,0.00036334913,0.000077892815,0.0029819245],"study_design_scores_gemma":[0.000005596723,0.000035916975,0.998187,0.0000031417294,0.000008572762,0.000115820185,0.00022527698,0.0006258777,0.00032688328,0.00012956039,0.00033192235,0.000004482437],"about_ca_topic_score_codex":0.004087567,"about_ca_topic_score_gemma":0.003982425,"teacher_disagreement_score":0.004087567,"about_ca_system_score_codex":0.0004942726,"about_ca_system_score_gemma":0.000092629365,"threshold_uncertainty_score":0.00812757},"labels":[],"label_agreement":null},{"id":"W1972554800","doi":"10.1088/0004-637x/726/2/77","title":"DISK GALAXY SCALING RELATIONS IN THE SFI++: INTRINSIC SCATTER AND APPLICATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Scaling; Astrophysics; Cepheid variable; Galaxy; Length scale; Luminosity; Constant (computer programming); Rotation (mathematics); Scale (ratio); Hubble's law; Geometry; Mathematics; Stars; Quantum mechanics","score_opus":0.005113722829755834,"score_gpt":0.2103306847362182,"score_spread":0.20521696190646235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972554800","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9674335,0.0014226012,0.02599701,0.00016354538,0.000014413195,0.000010233711,0.00081388943,0.000356705,0.003788202],"genre_scores_gemma":[0.9958812,0.00017376705,0.0030353155,0.00001937073,0.00003125027,0.0000043915984,0.00065369357,0.000055484976,0.00014560157],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99911684,0.00018686171,0.000045077282,0.0003513637,0.00024108295,0.000058836114],"domain_scores_gemma":[0.9899638,0.0044176946,0.002525557,0.0019025165,0.0008672624,0.00032307277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021457574,0.000520455,0.00045493172,0.0017923256,0.0003557956,0.0010076353,0.00059145916,0.00029088932,0.0010381542],"category_scores_gemma":[0.011716358,0.00018212872,0.00031094294,0.0023780998,0.00088635535,0.0009260962,0.000888173,0.00047588718,0.00037754918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049536993,0.00001944247,0.95148826,0.000070987226,0.00011503842,0.0000799946,0.0006742786,0.007900897,0.0051998184,0.004496353,0.00064471934,0.029260615],"study_design_scores_gemma":[0.0000065128306,0.00006210952,0.9171039,0.00004339033,0.000044523807,0.0005065522,0.00024683782,0.06032872,0.004450963,0.0141163925,0.0030401293,0.000049876235],"about_ca_topic_score_codex":0.0028551572,"about_ca_topic_score_gemma":0.0022311744,"teacher_disagreement_score":0.0028551572,"about_ca_system_score_codex":0.0005893138,"about_ca_system_score_gemma":0.00017788536,"threshold_uncertainty_score":0.0113479495},"labels":[],"label_agreement":null},{"id":"W1972648720","doi":"10.1086/339741","title":"The Gravitational Lens CFRS 03.1077","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Elliptical galaxy; Galaxy; Gravitational lens; Redshift; Lenticular galaxy; RADIUS; Fundamental plane (elliptical galaxies); Position angle; Mass distribution; Gravitation","score_opus":0.01115432820062905,"score_gpt":0.2084982043282308,"score_spread":0.19734387612760174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972648720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.64511794,0.0036542297,0.0047851396,0.0013589896,0.00018315407,0.000084457264,0.0049138395,0.0012232341,0.33867902],"genre_scores_gemma":[0.97310966,0.0005723145,0.0038577442,0.0002984749,0.00008715513,0.000011034238,0.0025415358,0.0000599369,0.01946233],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972075,0.000029043793,0.000006096398,0.00006864868,0.00012289059,0.000052558575],"domain_scores_gemma":[0.99950624,0.000036035548,0.00014045564,0.00008612337,0.00013947695,0.000091571594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004083151,0.00033435988,0.0002245602,0.0013076912,0.00074920437,0.00088988285,0.00018860062,0.00037171683,0.006506948],"category_scores_gemma":[0.00062377105,0.00013190783,0.00017171916,0.00089965214,0.00035089575,0.00036796718,0.00039241178,0.00029702025,0.0018037235],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005614201,0.00009217815,0.32431725,0.00024968287,0.00022353676,0.0010992849,0.0013693158,0.002293124,0.09825176,0.15046176,0.13333793,0.28774273],"study_design_scores_gemma":[0.00005646515,0.00014338607,0.73968303,0.00006960596,0.000062240695,0.001859652,0.00037918723,0.0051687434,0.013802486,0.0085872095,0.230131,0.0000569591],"about_ca_topic_score_codex":0.06734088,"about_ca_topic_score_gemma":0.066723816,"teacher_disagreement_score":0.06734088,"about_ca_system_score_codex":0.0025078251,"about_ca_system_score_gemma":0.0008835655,"threshold_uncertainty_score":0.13389784},"labels":[],"label_agreement":null},{"id":"W1972668755","doi":"10.1088/0004-637x/717/2/1123","title":"LOCATING PLANETESIMAL BELTS IN THE MULTIPLE-PLANET SYSTEMS HD 128311, HD 202206, HD 82943, AND HR 8799","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Planetesimal; Planet; Planetary system; Stars; Debris disk; Physics; Radiative transfer; Astrophysics; Astronomy; Giant planet; Astrobiology","score_opus":0.009521956143875117,"score_gpt":0.2145355809793999,"score_spread":0.2050136248355248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972668755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993562,0.0000213687,0.000111963345,0.000010689583,4.5506025e-7,0.0000012958664,0.00004177497,0.0000045824263,0.00045174125],"genre_scores_gemma":[0.99943036,0.000018810588,0.0002888543,0.000002913528,8.056252e-7,0.0000012529517,0.000114501774,0.0000012543661,0.00014114402],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999293,0.000010197389,0.0000037466796,0.000024174435,0.000018037996,0.0000146093],"domain_scores_gemma":[0.9997805,0.000037871818,0.000092733724,0.00001859286,0.000020806143,0.000049541355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014554955,0.00012495088,0.00013169668,0.0008871969,0.0004402372,0.00043454827,0.00030123262,0.000263004,0.0010466216],"category_scores_gemma":[0.00063050265,0.00010606414,0.000118783886,0.00064783037,0.00025304971,0.0003669102,0.0005131141,0.00012065103,0.0002409388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013639238,0.000046206536,0.95941263,0.000020410713,0.000021687674,0.0005694583,0.0005427304,0.0038625256,0.024765996,0.0006679264,0.00029528124,0.009658773],"study_design_scores_gemma":[0.000020265688,0.00005424952,0.9795593,0.000012903393,0.000018277071,0.000895416,0.0006213919,0.014624467,0.002880775,0.0005349749,0.0007650931,0.000012913476],"about_ca_topic_score_codex":0.012339179,"about_ca_topic_score_gemma":0.030450506,"teacher_disagreement_score":0.012339179,"about_ca_system_score_codex":0.00039530036,"about_ca_system_score_gemma":0.00022256508,"threshold_uncertainty_score":0.024534702},"labels":[],"label_agreement":null},{"id":"W1972677712","doi":"10.1086/500800","title":"δ Ceti Is Not Monoperiodic: Seismic Modeling of a β Cephei Star from<i>MOST</i>Space‐based Photometry","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Saint Mary's University; St. Mary's University; University of British Columbia","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Overtone; Stars; Asteroseismology; Oscillation (cell signaling); Light curve; Duty cycle; Surface gravity; Variable star; Astronomy; Spectral line","score_opus":0.013471514145791041,"score_gpt":0.22217891030543613,"score_spread":0.2087073961596451,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972677712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98492265,0.00008683094,0.0028027876,0.00037618083,0.000029229372,0.000012500359,0.000933957,0.0002267229,0.010609145],"genre_scores_gemma":[0.9983804,0.000026160556,0.0005741144,0.000025626761,0.0000052914334,0.00000293337,0.00039300474,0.000043559427,0.0005489091],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999684,0.0000023442522,0.0000013041433,0.000013473114,0.0000052752416,0.00000919252],"domain_scores_gemma":[0.9998373,0.000025295685,0.000021781447,0.00001585532,0.00003177459,0.00006791216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001108975,0.0002741871,0.00022193485,0.00027352732,0.00049157965,0.0006317264,0.00059248094,0.0006709344,0.0027895733],"category_scores_gemma":[0.00042635942,0.00027906056,0.00024589946,0.00044668032,0.00026587033,0.00030872133,0.00027702918,0.00062046637,0.00066977926],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078555814,0.00036950223,0.18497424,0.00012368202,0.00012484743,0.0017551807,0.0006314328,0.73635906,0.029787444,0.009133998,0.010254353,0.02570074],"study_design_scores_gemma":[0.00006629237,0.000074181866,0.074595936,0.000011123593,0.000033870172,0.00019276852,0.00020773732,0.9205393,0.0014561531,0.0013168101,0.001478007,0.000027852711],"about_ca_topic_score_codex":0.0288557,"about_ca_topic_score_gemma":0.022692056,"teacher_disagreement_score":0.0288557,"about_ca_system_score_codex":0.0004639547,"about_ca_system_score_gemma":0.0006555357,"threshold_uncertainty_score":0.05737549},"labels":[],"label_agreement":null},{"id":"W1972727650","doi":"10.1088/0004-637x/754/1/28","title":"[Fe III] EMISSION LINES IN THE PLANETARY NEBULA NGC 2392","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Nebula; Emission nebula; Spectral line; Emission spectrum; Protoplanetary nebula","score_opus":0.01424491051528999,"score_gpt":0.23727913380279808,"score_spread":0.2230342232875081,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972727650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987447,0.000052105454,0.00018935784,0.000009108171,0.0000011552615,0.0000014143577,0.00005042774,0.00002202151,0.0009295607],"genre_scores_gemma":[0.99951077,0.000023751893,0.00023618298,0.0000041004005,0.000001950987,0.0000014708928,0.000100107885,0.000003176271,0.00011855397],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995375,0.0000034913492,0.0000016090182,0.000019359304,0.00001250912,0.000009345045],"domain_scores_gemma":[0.9999224,0.000006553008,0.000027818494,0.0000057761135,0.000008737747,0.000028815724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000067723544,0.00022736787,0.0001415275,0.0006200889,0.000386089,0.00039496078,0.00022872444,0.0002943453,0.00064116303],"category_scores_gemma":[0.00016091716,0.00016471907,0.00017437548,0.00033862848,0.00024197155,0.00020758125,0.0002743223,0.0001378472,0.00014652264],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025262346,0.00010360035,0.7115333,0.00003324302,0.00010470486,0.0028783393,0.00042687557,0.0068803183,0.2661358,0.0010200377,0.00045974265,0.010171269],"study_design_scores_gemma":[0.000017383034,0.0000546928,0.98472136,0.000005631408,0.00002317381,0.00092159054,0.0001632771,0.0069196434,0.0053010564,0.00057285104,0.001282712,0.000016561353],"about_ca_topic_score_codex":0.0071614324,"about_ca_topic_score_gemma":0.0065185106,"teacher_disagreement_score":0.0071614324,"about_ca_system_score_codex":0.00034612423,"about_ca_system_score_gemma":0.00010898105,"threshold_uncertainty_score":0.01423949},"labels":[],"label_agreement":null},{"id":"W1972755417","doi":"10.1088/0004-637x/704/2/1657","title":"PATTERN SPEEDS OF BARS AND SPIRAL ARMS FROM Hα VELOCITY FIELDS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Spiral galaxy; Astrophysics; Bar (unit); RADIUS; Galaxy; Velocity dispersion; Spiral (railway); Photometry (optics); Geometry; Stars; Mathematical analysis; Mathematics","score_opus":0.007508618266155758,"score_gpt":0.2085279141245563,"score_spread":0.20101929585840053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972755417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9753897,0.000047895817,0.023001451,0.00000988536,0.000004916149,0.000021483613,0.00033363028,0.00021845616,0.0009726028],"genre_scores_gemma":[0.9745634,0.000028929062,0.024607625,0.0000030603603,0.0000029192443,0.000015528352,0.00038495753,0.000044816206,0.0003487588],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997558,0.000045679175,0.000018495506,0.00010109733,0.00005434271,0.000024657535],"domain_scores_gemma":[0.9988451,0.00041220256,0.0002598502,0.00018578414,0.00023907951,0.00005796925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006870915,0.00028372128,0.00021002801,0.0017537745,0.00019383225,0.00053413917,0.00036908578,0.00017902062,0.000897551],"category_scores_gemma":[0.0032925773,0.00023136192,0.00022149178,0.00067886914,0.00020903152,0.0003950263,0.00030455462,0.00018708414,0.0003217778],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004227106,0.00009855413,0.57969165,0.00015310172,0.0002195881,0.000305565,0.0008696505,0.16891089,0.07976552,0.0032939801,0.00048693706,0.1657819],"study_design_scores_gemma":[0.00003601778,0.00013682527,0.3931948,0.000020167066,0.0000436748,0.0002202124,0.00014247143,0.5632612,0.039499406,0.002130583,0.0012544333,0.000060196373],"about_ca_topic_score_codex":0.00511686,"about_ca_topic_score_gemma":0.0066660102,"teacher_disagreement_score":0.00511686,"about_ca_system_score_codex":0.00049496896,"about_ca_system_score_gemma":0.00026222132,"threshold_uncertainty_score":0.010174155},"labels":[],"label_agreement":null},{"id":"W1972763344","doi":"10.1086/587928","title":"The Redshift Evolution of Wet, Dry, and Mixed Galaxy Mergers from Close Galaxy Pairs in the DEEP2 Galaxy Redshift Survey","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":238,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University","funders":"","keywords":"Astrophysics; Physics; Galaxy merger; Redshift; Astronomy; Galaxy; Redshift survey; Luminous infrared galaxy; Merge (version control)","score_opus":0.01117837415446589,"score_gpt":0.2134890862826951,"score_spread":0.2023107121282292,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972763344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991602,0.000086873784,0.00013323307,0.000013914552,6.2806055e-7,0.0000016726127,0.00032234,0.000010068567,0.0002710929],"genre_scores_gemma":[0.99885046,0.000039966835,0.00012282109,0.0000064105625,0.0000017922571,0.0000015983835,0.00085742894,0.000003914112,0.000115668714],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996264,0.0000762762,0.000021247171,0.000099795165,0.00007425985,0.00010203107],"domain_scores_gemma":[0.9973091,0.00045114572,0.0013234632,0.00019378673,0.00021958096,0.00050296274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007356436,0.00034825646,0.0003032416,0.0022081975,0.00030787513,0.00090215914,0.0003358214,0.00035277728,0.00097121095],"category_scores_gemma":[0.002666352,0.00033576024,0.00037998342,0.0015619439,0.00035961423,0.0007396459,0.001260649,0.00030552744,0.0002515031],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000069766524,0.000009619293,0.99486923,0.00000861189,0.00005059003,0.000055780914,0.00018513908,0.00055753737,0.0018909848,0.00018017292,0.0000945524,0.0020280431],"study_design_scores_gemma":[0.0000018042199,0.000013284613,0.99865025,0.0000017425122,0.000008522178,0.00006944733,0.00008715998,0.0007562061,0.0001990991,0.000044919587,0.00016412468,0.000003414723],"about_ca_topic_score_codex":0.008527632,"about_ca_topic_score_gemma":0.011062541,"teacher_disagreement_score":0.008527632,"about_ca_system_score_codex":0.0004613052,"about_ca_system_score_gemma":0.00011732565,"threshold_uncertainty_score":0.016955972},"labels":[],"label_agreement":null},{"id":"W1972828295","doi":"10.1086/337958","title":"New X‐Ray Clusters in the<i>Einstein</i>Extended Medium Sensitivity Survey. II. Optical Properties","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Surface brightness; Galaxy cluster; Galaxy; Redshift; Cluster (spacecraft); Brightness; Galaxy groups and clusters; Cosmology; Astronomy; Sensitivity (control systems)","score_opus":0.01625273273595997,"score_gpt":0.20578997844205205,"score_spread":0.18953724570609207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972828295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99409616,0.00068952097,0.00026130065,0.00009176173,0.000010545722,0.000021698075,0.0021923466,0.000033266748,0.0026033071],"genre_scores_gemma":[0.9894052,0.00043403654,0.0014388538,0.000072319075,0.000012769823,0.000018518034,0.0059434855,0.00001310358,0.0026617364],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978167,0.000009035835,0.000009127884,0.0000453183,0.000088438144,0.000066430934],"domain_scores_gemma":[0.99952126,0.00002376662,0.00013786236,0.000045665583,0.0001223993,0.00014905978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021355032,0.00015051012,0.00015884193,0.0011347272,0.0006192054,0.0005531623,0.0003057075,0.0001242403,0.0012897815],"category_scores_gemma":[0.0004764757,0.00018068148,0.0001557906,0.0011331355,0.0002747141,0.00032924936,0.0006657312,0.0002009827,0.00025104696],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001909851,0.000030271533,0.96410143,0.000050697214,0.00006713273,0.00026564504,0.000790615,0.00030498963,0.0054638786,0.00084992475,0.0037983372,0.024086075],"study_design_scores_gemma":[0.0000022629652,0.0000064123246,0.9960407,0.0000032592884,0.000007853548,0.000098480625,0.00010348652,0.00006013602,0.00011736875,0.000028188302,0.0035292907,0.0000023917728],"about_ca_topic_score_codex":0.20290722,"about_ca_topic_score_gemma":0.48351243,"teacher_disagreement_score":0.20290722,"about_ca_system_score_codex":0.0012062019,"about_ca_system_score_gemma":0.00071036094,"threshold_uncertainty_score":0.40345228},"labels":[],"label_agreement":null},{"id":"W1972830263","doi":"10.1086/513687","title":"The Kinetic Sunyaev‐Zel’dovich Effect from Radiative Transfer Simulations of Patchy Reionization","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; Physics; Astrophysics; Sunyaev–Zel'dovich effect; Cosmic microwave background; Dark Ages; South Pole Telescope; Radiative transfer; Redshift; Galaxy; Anisotropy; Optics","score_opus":0.004566881032393491,"score_gpt":0.21399604972992517,"score_spread":0.20942916869753167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1972830263","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97173554,0.0001276539,0.016222648,0.00027914552,0.00003418687,0.000037147875,0.00046167528,0.00038503352,0.010717078],"genre_scores_gemma":[0.99599373,0.00006787437,0.0024850236,0.000058833655,0.000017483057,0.00003085744,0.0002284453,0.00016697802,0.00095081935],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998417,0.000036977453,0.000005773087,0.000021448106,0.000035940062,0.000058148515],"domain_scores_gemma":[0.9988194,0.0006939119,0.00016288809,0.000079850455,0.00010300112,0.00014092782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003918139,0.00066558557,0.00055138493,0.0003909708,0.00035085075,0.00063774927,0.0010003814,0.00065962155,0.002623716],"category_scores_gemma":[0.002555347,0.0004287597,0.0006804895,0.0005577684,0.0005856653,0.00050027936,0.00065884937,0.00078225863,0.00019082498],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057078058,0.000022347826,0.002255242,0.000019007111,0.000026847869,0.00007461996,0.000029082059,0.9927061,0.0019446688,0.0016218104,0.00019288037,0.0010503349],"study_design_scores_gemma":[0.00002701616,0.000012746473,0.0012692275,0.0000015959787,0.0000057273414,0.000008436167,0.0000085416605,0.9975217,0.00058480114,0.0004416433,0.000113494796,0.0000050442777],"about_ca_topic_score_codex":0.016348867,"about_ca_topic_score_gemma":0.0059921704,"teacher_disagreement_score":0.016348867,"about_ca_system_score_codex":0.0010408118,"about_ca_system_score_gemma":0.0006409153,"threshold_uncertainty_score":0.03250742},"labels":[],"label_agreement":null},{"id":"W1973114600","doi":"10.1086/428384","title":"Limits on the Polarization of the Cosmic Microwave Background Radiation at Multipoles up to<i>l</i>∼ 2000","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Polarization (electrochemistry); Cassegrain reflector; Interferometry; Cosmic background radiation; Radiation; Background radiation; Microwave","score_opus":0.01085403703215573,"score_gpt":0.23861857495443733,"score_spread":0.2277645379222816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973114600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9157543,0.005703962,0.032516107,0.000996224,0.000044080938,0.000046022382,0.0042699617,0.0009848106,0.039684486],"genre_scores_gemma":[0.98644245,0.0011185143,0.0056979284,0.00030360807,0.00010918233,0.00008644978,0.004959306,0.000103983984,0.0011785902],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99912685,0.00015707604,0.00003717557,0.00018797819,0.0002205107,0.00027047002],"domain_scores_gemma":[0.99264115,0.0043032644,0.0014189957,0.00075292896,0.0004531915,0.0004303691],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021675085,0.00080695166,0.0004235705,0.0019642883,0.00055427913,0.0017633152,0.00076386344,0.00078697345,0.003196949],"category_scores_gemma":[0.004534078,0.00052909605,0.00055946613,0.0009981295,0.00086454186,0.0013589142,0.0014859821,0.0012490852,0.0011271519],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004239187,0.0005920956,0.6416418,0.0011439116,0.0004132134,0.0010795406,0.0014917485,0.028288765,0.13184673,0.025015958,0.012439739,0.15180731],"study_design_scores_gemma":[0.00017578459,0.00036401817,0.82594556,0.0004445427,0.0002460598,0.00092222926,0.00033300012,0.031533085,0.08028965,0.019471746,0.04009775,0.0001764551],"about_ca_topic_score_codex":0.0025540628,"about_ca_topic_score_gemma":0.0024967538,"teacher_disagreement_score":0.003196949,"about_ca_system_score_codex":0.001277843,"about_ca_system_score_gemma":0.00042117524,"threshold_uncertainty_score":0.0114629865},"labels":[],"label_agreement":null},{"id":"W1973209257","doi":"10.1086/318242","title":"Gravitational Lensing by Galaxy Groups in the Hubble Deep Field","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Hubble Deep Field; Gravitational lens; Galaxy; Hubble Ultra-Deep Field; Strong gravitational lensing; Galaxy group; Weak gravitational lensing; Hubble's law; Elliptical galaxy; Hubble Deep Field South","score_opus":0.007577075974644067,"score_gpt":0.21818179557305892,"score_spread":0.21060471959841484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973209257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990928,0.00012221845,0.00017728849,0.000019107245,6.6206553e-7,0.000001967355,0.00004500979,0.000003233712,0.00053779996],"genre_scores_gemma":[0.9992374,0.00012885357,0.00022085545,0.0000073271626,0.000004600477,0.0000013327717,0.0000924153,0.0000012026566,0.0003058908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975246,0.00006287788,0.000007564781,0.000032441854,0.000053792868,0.000090994276],"domain_scores_gemma":[0.9971349,0.0010782816,0.0009876136,0.00019098385,0.0000924901,0.00051563967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00075364433,0.00042883406,0.00024946575,0.0015355701,0.0004554125,0.0006985802,0.00027270033,0.00026547164,0.0010094105],"category_scores_gemma":[0.002691375,0.00019201593,0.00024317697,0.0012787002,0.00067541504,0.0008014254,0.0006660342,0.00023816786,0.00013669011],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010352829,0.00028032975,0.93538004,0.000094123556,0.00024322626,0.0005165328,0.0009032726,0.013019816,0.015509971,0.008126411,0.0008034723,0.024087517],"study_design_scores_gemma":[0.00007668998,0.0004554506,0.9628443,0.000024197576,0.00011660274,0.00045649076,0.00088281045,0.022039356,0.004861845,0.006684196,0.0015242044,0.000033851848],"about_ca_topic_score_codex":0.017924553,"about_ca_topic_score_gemma":0.021917598,"teacher_disagreement_score":0.017924553,"about_ca_system_score_codex":0.0009005676,"about_ca_system_score_gemma":0.00023230269,"threshold_uncertainty_score":0.03564042},"labels":[],"label_agreement":null},{"id":"W1973311828","doi":"10.1086/422636","title":"Discovery of a Transient Magnetar: XTE J1810-197","year":2004,"lang":"it","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":237,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; McGill University","funders":"","keywords":"Magnetar; Pulsar; Physics; Astrophysics; Neutron star; X-ray pulsar; Vela; Flux (metallurgy); RADIUS; ROSAT; Astronomy; Galaxy","score_opus":0.01092654725812597,"score_gpt":0.28754004576089587,"score_spread":0.2766134985027699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973311828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99652183,0.00061739126,0.00029649635,0.00021603859,0.0000638978,0.000011225535,0.00023715252,0.0000402255,0.0019957374],"genre_scores_gemma":[0.9948561,0.00064918894,0.00083629705,0.00029343943,0.00017742431,0.000015652973,0.0012177965,0.000011841452,0.0019422529],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999249,0.000003473398,0.000004669927,0.000022268057,0.000017472865,0.000027209286],"domain_scores_gemma":[0.9997397,0.000027126112,0.00009733244,0.000018095892,0.000024474939,0.000093230854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011053252,0.00022739974,0.00022886427,0.0005204575,0.0005780364,0.0009959808,0.00047418708,0.0006331767,0.0010820528],"category_scores_gemma":[0.0002375748,0.00015925153,0.00014488242,0.00036579432,0.00047538348,0.00037014217,0.00061359024,0.00042928418,0.00050860405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013853523,0.0004958855,0.586563,0.0002971299,0.00014954957,0.08226668,0.0010446153,0.0003480874,0.25959817,0.0017769048,0.006772213,0.059302453],"study_design_scores_gemma":[0.00014325045,0.0013603284,0.7972626,0.000080423764,0.00016594207,0.085521296,0.0008794355,0.0013238611,0.046830244,0.0007215581,0.06564865,0.00006242335],"about_ca_topic_score_codex":0.0012483603,"about_ca_topic_score_gemma":0.0022769882,"teacher_disagreement_score":0.0012483603,"about_ca_system_score_codex":0.00043509458,"about_ca_system_score_gemma":0.00022971336,"threshold_uncertainty_score":0.0036198497},"labels":[],"label_agreement":null},{"id":"W1973331810","doi":"10.1086/498210","title":"The ACS Virgo Cluster Survey. IX. The Color Distributions of Globular Cluster Systems in Early‐Type Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":444,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Globular cluster; Virgo Cluster; Galaxy; Metallicity; Dwarf galaxy; Astronomy; Elliptical galaxy; Luminosity; Galaxy cluster","score_opus":0.007476522499628624,"score_gpt":0.212638554484144,"score_spread":0.20516203198451538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973331810","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.19132839,0.002360655,0.0016445362,0.0006005091,0.00011183666,0.00021773884,0.7563461,0.00340011,0.043990154],"genre_scores_gemma":[0.24613705,0.0013071446,0.0043750866,0.00027820034,0.00010195681,0.00015450512,0.7309619,0.00037813224,0.016306074],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998072,0.000019937852,0.0000129818145,0.000044903227,0.00006780534,0.000047213667],"domain_scores_gemma":[0.99942565,0.000033279644,0.00014663672,0.00006998799,0.00018371452,0.00014075058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004552994,0.00061214814,0.00034389633,0.0051251827,0.00030156306,0.00085101,0.00058850134,0.00028120307,0.010695343],"category_scores_gemma":[0.0009378175,0.00018999311,0.00031837448,0.005181401,0.00013150707,0.00045080413,0.00092246704,0.00035888355,0.0068794563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037504424,0.00013138025,0.525797,0.00044713946,0.00036098933,0.00015676857,0.0003737845,0.00093230844,0.0038375934,0.0026793238,0.38455284,0.08035582],"study_design_scores_gemma":[0.00004678265,0.000023693283,0.90316135,0.000037689486,0.0000370786,0.00009347152,0.0001223976,0.00052280055,0.00041043974,0.00038328418,0.09514891,0.0000120182385],"about_ca_topic_score_codex":0.04770847,"about_ca_topic_score_gemma":0.03809511,"teacher_disagreement_score":0.04770847,"about_ca_system_score_codex":0.00082938216,"about_ca_system_score_gemma":0.00046588093,"threshold_uncertainty_score":0.09486157},"labels":[],"label_agreement":null},{"id":"W1973345745","doi":"10.1086/344106","title":"Interferometric Observations of the Nuclear Region of Arp 220 at Submillimeter Wavelengths","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"James Clerk Maxwell Telescope; Redshift; Interferometry; Wavelength; Line (geometry); Infrared; Binary number; Emission spectrum; Telescope; Observatory","score_opus":0.022375633960163076,"score_gpt":0.19742883190607646,"score_spread":0.1750531979459134,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973345745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99580413,0.00022617764,0.0007209526,0.000026133492,0.0000066790653,0.0000072244916,0.00023492593,0.00010258652,0.002871232],"genre_scores_gemma":[0.99717146,0.000121343866,0.0015075322,0.000045127712,0.000023321962,0.000010626312,0.0008359602,0.000015987745,0.00026882318],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998572,0.000012887577,0.000005590258,0.00003713543,0.000050580195,0.0000365861],"domain_scores_gemma":[0.99968565,0.000039190676,0.00011528529,0.00004407402,0.000038204922,0.00007767388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021896198,0.00027472823,0.00023322922,0.00092017814,0.000501197,0.0006417478,0.0003945079,0.00024565903,0.00044291563],"category_scores_gemma":[0.0004942495,0.00033024212,0.000225018,0.00044950863,0.00021102566,0.00036125377,0.000575237,0.00038200358,0.00024557544],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045529215,0.00032757173,0.605877,0.00012904446,0.00029932545,0.0009183446,0.0012130777,0.0016635703,0.33462328,0.00091298117,0.0015445021,0.052035954],"study_design_scores_gemma":[0.000019403293,0.00018846703,0.9829685,0.000011859026,0.00007893198,0.00051698193,0.00018723539,0.0016955079,0.009145986,0.00018727576,0.0049808524,0.00001901976],"about_ca_topic_score_codex":0.001964022,"about_ca_topic_score_gemma":0.004664959,"teacher_disagreement_score":0.001964022,"about_ca_system_score_codex":0.0003532976,"about_ca_system_score_gemma":0.00017522152,"threshold_uncertainty_score":0.003905177},"labels":[],"label_agreement":null},{"id":"W1973396674","doi":"10.1086/426309","title":"Colliding Winds in Symbiotic Binary Systems. I. Analytic and Numerical Solutions","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Royal Military College of Canada","funders":"","keywords":"Physics; Radiative transfer; Adiabatic process; Symbiotic star; Radiative cooling; Stars; Binary number; Astrophysics; Astronomy; Quantum mechanics","score_opus":0.011540296820703164,"score_gpt":0.22338226976904554,"score_spread":0.2118419729483424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973396674","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2008458,0.008087533,0.6929381,0.0022931409,0.00057983695,0.0002284336,0.00043104557,0.00040713605,0.09418904],"genre_scores_gemma":[0.8195464,0.0045624934,0.15318196,0.0003844966,0.00035233542,0.0005390151,0.00035419292,0.00020792191,0.02087123],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981993,0.0000631177,0.000010173884,0.000013936986,0.000063857326,0.000029002193],"domain_scores_gemma":[0.9995414,0.00018890713,0.00009928595,0.000029203215,0.00010020762,0.000041084593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004913037,0.0005545005,0.000514201,0.0006287367,0.00063867593,0.0010758404,0.0010260933,0.0014487416,0.002920545],"category_scores_gemma":[0.004157432,0.0003817238,0.0005033845,0.00062175834,0.0007858618,0.0011069499,0.0014591396,0.0007787172,0.0004526342],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022577833,0.00004288252,0.0021038342,0.00012534397,0.000025334512,0.00035862796,0.00030686456,0.613015,0.0013397299,0.36625573,0.0021520243,0.014252082],"study_design_scores_gemma":[0.000015782036,0.0000073455676,0.00024381359,0.000020994978,0.000004082412,0.00006198819,0.00006472813,0.93914485,0.00010487062,0.05666496,0.0036593636,0.000007191273],"about_ca_topic_score_codex":0.0060607153,"about_ca_topic_score_gemma":0.0041806237,"teacher_disagreement_score":0.0060607153,"about_ca_system_score_codex":0.0011050397,"about_ca_system_score_gemma":0.00067443604,"threshold_uncertainty_score":0.012050867},"labels":[],"label_agreement":null},{"id":"W1973451030","doi":"10.1086/587771","title":"Gemini Imaging of Mid‐Infrared Emission from the Nuclear Region of Centaurus A","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Centaurus A; Physics; Astrophysics; Torus; Emission spectrum; Infrared; Line (geometry); Luminous infrared galaxy; Synchrotron; Active galactic nucleus; Astronomy; Galaxy; Spectral line; Optics; Geometry","score_opus":0.012725524470261403,"score_gpt":0.22115695808001667,"score_spread":0.20843143360975527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973451030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9705493,0.00096139085,0.0017658569,0.0009448206,0.00017774821,0.000026591548,0.0014508443,0.00056489237,0.023558639],"genre_scores_gemma":[0.9869034,0.00028872624,0.0022799408,0.00016689567,0.00014419381,0.000011861777,0.0015036563,0.000105595704,0.008595681],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991214,0.0000058728974,0.0000032288972,0.000024425035,0.00003071628,0.000023527844],"domain_scores_gemma":[0.99970514,0.00002343216,0.00003656648,0.000034897308,0.00008538902,0.00011446129],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003165075,0.00013965138,0.00018744536,0.00073363545,0.0008112577,0.0006294894,0.0002444807,0.00045552163,0.006083793],"category_scores_gemma":[0.00037080015,0.00018359507,0.00014183526,0.00043736713,0.00017603186,0.00047673075,0.0005169745,0.00036172246,0.0012881978],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016078855,0.00013647144,0.10426936,0.0002823426,0.00006789769,0.0010470202,0.0008545627,0.0004345023,0.8134548,0.001464166,0.016674444,0.0597066],"study_design_scores_gemma":[0.000058922462,0.000165516,0.92317563,0.000028340792,0.00007159414,0.0010907557,0.00041758263,0.0018861241,0.045267925,0.00046220183,0.027348634,0.00002691348],"about_ca_topic_score_codex":0.0019042968,"about_ca_topic_score_gemma":0.005232856,"teacher_disagreement_score":0.006083793,"about_ca_system_score_codex":0.0002831881,"about_ca_system_score_gemma":0.00018441037,"threshold_uncertainty_score":0.020352304},"labels":[],"label_agreement":null},{"id":"W1973468734","doi":"10.1088/0004-637x/779/2/136","title":"THE RELATIVE ROLE OF GALAXY MERGERS AND COSMIC FLOWS IN FEEDING BLACK HOLES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Supermassive black hole; Galaxy; Halo; Angular momentum; Black hole (networking); Galaxy formation and evolution; Accretion (finance); Specific relative angular momentum","score_opus":0.005248602546607254,"score_gpt":0.19624425296779008,"score_spread":0.19099565042118283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973468734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99862397,0.000083862215,0.00040442796,0.00007148675,0.000004646032,0.0000061438727,0.00010769066,0.000021082948,0.00067663507],"genre_scores_gemma":[0.9992079,0.000052964024,0.00047466165,0.000019200656,0.0000038862127,0.000003984568,0.00010018795,0.000012551525,0.00012457394],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998399,0.000059131693,0.0000076293327,0.000031932694,0.000015649686,0.000045768404],"domain_scores_gemma":[0.998838,0.0005043072,0.00022159172,0.00005904895,0.000049179827,0.00032783663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008237024,0.00059377716,0.00043496332,0.0008367335,0.0008769091,0.0014490265,0.00093251123,0.0009342952,0.001423363],"category_scores_gemma":[0.0047068708,0.0005890766,0.00056691945,0.00056023186,0.0010512623,0.001124112,0.00088725233,0.0007336218,0.000117246236],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009305703,0.00030234424,0.275001,0.00009099855,0.00033686825,0.00043137438,0.0004573389,0.70181036,0.0069847275,0.00867362,0.0005713155,0.0044095563],"study_design_scores_gemma":[0.00022500247,0.00022742036,0.09047113,0.000028901677,0.00013500606,0.00009321873,0.00036909673,0.9032728,0.0013938323,0.0032653355,0.0004690814,0.000049101087],"about_ca_topic_score_codex":0.032597136,"about_ca_topic_score_gemma":0.035408907,"teacher_disagreement_score":0.032597136,"about_ca_system_score_codex":0.0013549576,"about_ca_system_score_gemma":0.0007311054,"threshold_uncertainty_score":0.064814806},"labels":[],"label_agreement":null},{"id":"W1973475010","doi":"10.1086/426576","title":"Spatially Resolved Spectroscopy of the<i>Chandra</i>Field Containing the Supernova Remnant G292.2−0.5","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; McGill University; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Physics; Supernova remnant; Pulsar; Astrophysics; Pulsar wind nebula; Nebula; Astronomy; Point source; Photon; Supernova; Stars; Optics","score_opus":0.008320800910181088,"score_gpt":0.22507079198416716,"score_spread":0.21674999107398607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973475010","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970445,0.00024269143,0.00039950234,0.000033939097,0.0000073598776,0.0000107221085,0.0002742467,0.00006741136,0.0019195864],"genre_scores_gemma":[0.99646735,0.00018188417,0.0018516178,0.00006626555,0.00002269868,0.000013386283,0.0010202266,0.000019859239,0.00035669038],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993587,0.000004642677,0.0000025429438,0.000019534398,0.00001594517,0.000021468217],"domain_scores_gemma":[0.9997863,0.000023683651,0.000057394493,0.00002957006,0.000028398517,0.00007458027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015824311,0.0002483899,0.00021723787,0.0006627151,0.00039588733,0.00028234025,0.000399282,0.00020241216,0.0006759021],"category_scores_gemma":[0.0001834054,0.00016728212,0.00022577017,0.00046063183,0.00023029365,0.00019006197,0.0004424365,0.00033526446,0.00021582466],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083630043,0.00031056022,0.101815455,0.00014229021,0.00015116799,0.0021176466,0.0003058014,0.0012881787,0.8778446,0.00065562583,0.0011521531,0.013380118],"study_design_scores_gemma":[0.000056427925,0.00032793914,0.95891637,0.00002100283,0.00007046774,0.0018109871,0.00014732119,0.002118627,0.033097684,0.00025807365,0.0031467793,0.000028309254],"about_ca_topic_score_codex":0.0019808863,"about_ca_topic_score_gemma":0.0034964404,"teacher_disagreement_score":0.0019808863,"about_ca_system_score_codex":0.00020866234,"about_ca_system_score_gemma":0.00016695035,"threshold_uncertainty_score":0.0039387345},"labels":[],"label_agreement":null},{"id":"W1973500133","doi":"10.1088/0004-637x/743/2/143","title":"TESTING SCALING RELATIONS FOR SOLAR-LIKE OSCILLATIONS FROM THE MAIN SEQUENCE TO RED GIANTS USING<i>KEPLER</i>DATA","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":408,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Amplitude; Stars; Scaling; Subgiant; Oscillation (cell signaling); Hertzsprung–Russell diagram; Instability strip; Asteroseismology; Main sequence; Astronomy; Stellar evolution; Cepheid variable; Geometry","score_opus":0.13393060435988202,"score_gpt":0.28871502693325624,"score_spread":0.15478442257337421,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973500133","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99652725,0.0000643963,0.0012067792,0.00013501744,0.000020672449,0.000009034768,0.00047724805,0.00004409319,0.0015154225],"genre_scores_gemma":[0.99861276,0.000021236378,0.00048481039,0.0000168167,0.00001807394,0.000006344575,0.00071045506,0.00003467724,0.00009471893],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998747,0.00047037806,0.00009599094,0.00046419495,0.00012592155,0.00009651057],"domain_scores_gemma":[0.9415797,0.045644876,0.0045469673,0.003749526,0.0026975933,0.0017813229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003509907,0.0005606715,0.0003216677,0.0014749961,0.00092654687,0.0016517233,0.0006940726,0.0006498973,0.0042376397],"category_scores_gemma":[0.034764726,0.00023600191,0.0009002519,0.0013622852,0.00081694167,0.0019516281,0.00092459255,0.00086601486,0.00064026087],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062567863,0.00016998895,0.9529791,0.00009285083,0.00055145955,0.0002570431,0.0017139058,0.0066213566,0.0070075695,0.0026063581,0.0017321057,0.025642563],"study_design_scores_gemma":[0.00010512043,0.0003049536,0.95758367,0.000037320835,0.00023341479,0.00020398777,0.0019883283,0.031721078,0.0015702638,0.0049346243,0.0012781144,0.000039123614],"about_ca_topic_score_codex":0.009402227,"about_ca_topic_score_gemma":0.005958744,"teacher_disagreement_score":0.009402227,"about_ca_system_score_codex":0.0004689021,"about_ca_system_score_gemma":0.0003930771,"threshold_uncertainty_score":0.018694997},"labels":[],"label_agreement":null},{"id":"W1973503998","doi":"10.1086/308522","title":"The Search for Primordial<sup>3</sup>He Using the 8.665 GHz Hyperfine Spin‐Flip Transition of<sup>3</sup>He<sup>+</sup>","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Galaxy; Astrophysics; Hyperfine structure; Galactic Center; RADIUS; Atomic physics","score_opus":0.0194486979877046,"score_gpt":0.2674430956048178,"score_spread":0.24799439761711323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973503998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982322,0.00022774136,0.0008199534,0.000019366194,0.0000018051613,0.000004800414,0.000052262352,0.00001087083,0.0006311045],"genre_scores_gemma":[0.99836594,0.00011290656,0.0011355273,0.000020747677,0.0000040739747,0.0000034360232,0.00012795185,0.000002288263,0.00022717747],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995613,0.0000047840217,0.000001714207,0.000017023136,0.000009174644,0.000011189382],"domain_scores_gemma":[0.9998141,0.000026447293,0.000088376764,0.000021382364,0.00001581329,0.000033887245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015778025,0.00019683206,0.00009184286,0.00033067563,0.00017781396,0.00029708707,0.0002584082,0.0003101276,0.00058199983],"category_scores_gemma":[0.00019142694,0.000159286,0.00012251946,0.00025313176,0.00021643384,0.00025794026,0.00022177916,0.00019511709,0.00017292042],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035346785,0.00003127184,0.39537778,0.000065317785,0.00006848426,0.00033597092,0.00021396321,0.00019823211,0.5869021,0.00054656155,0.00008188382,0.015824901],"study_design_scores_gemma":[0.000012371901,0.0001790606,0.94454306,0.000007800322,0.00003167584,0.00056612777,0.00012333572,0.00096169225,0.05203901,0.00027927707,0.0012483725,0.000008244167],"about_ca_topic_score_codex":0.0009945518,"about_ca_topic_score_gemma":0.0017168376,"teacher_disagreement_score":0.0009945518,"about_ca_system_score_codex":0.00015033098,"about_ca_system_score_gemma":0.000087760964,"threshold_uncertainty_score":0.001977563},"labels":[],"label_agreement":null},{"id":"W1973541959","doi":"10.1086/505644","title":"Implications of <i>WMAP</i> 3 Year Data for the Sources of Reionization","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; CMB cold spot; Cosmic microwave background; Physics; Astrophysics; Redshift; Stars; Star formation; Astronomy; Anisotropy; Galaxy","score_opus":0.013285588674144758,"score_gpt":0.26320690545559583,"score_spread":0.24992131678145107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973541959","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79324436,0.009923035,0.02583118,0.09633617,0.0040876796,0.00007325159,0.029305896,0.0010375195,0.04016099],"genre_scores_gemma":[0.9725495,0.0020943463,0.0053621707,0.009793087,0.0012206676,0.00007274769,0.006701486,0.0001935374,0.002012487],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993469,0.00013636217,0.00007399438,0.00016486752,0.0001802121,0.00009766103],"domain_scores_gemma":[0.9908159,0.0036652945,0.002659875,0.0013952348,0.0008676509,0.00059606304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038946948,0.0006373452,0.00036097335,0.0016544146,0.00064741087,0.0025772082,0.0016975228,0.0015623724,0.0037690825],"category_scores_gemma":[0.0103682885,0.00034360748,0.0012373055,0.0021817342,0.0009930374,0.0025965367,0.0011349736,0.0027812344,0.00056501257],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014048589,0.00020866185,0.59166557,0.0006573672,0.001035596,0.004693368,0.001931045,0.019798676,0.018059738,0.17318475,0.11523502,0.07212544],"study_design_scores_gemma":[0.00014274546,0.0000667701,0.7478847,0.00037221634,0.00035985658,0.0018662608,0.0012255005,0.014302799,0.010829469,0.15184435,0.070769876,0.00033547377],"about_ca_topic_score_codex":0.016930794,"about_ca_topic_score_gemma":0.008723812,"teacher_disagreement_score":0.016930794,"about_ca_system_score_codex":0.0014278915,"about_ca_system_score_gemma":0.0007734004,"threshold_uncertainty_score":0.033664465},"labels":[],"label_agreement":null},{"id":"W1973559081","doi":"10.1086/504892","title":"The<sup>1</sup><i>D</i>–<sup>3</sup><i>P</i>Transitions in Atomic Oxygen Induced by Impact with Atomic Hydrogen","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Catalytic Processes in Materials Science","field":"Materials Science","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Atomic physics; Hydrogen; Excitation; Oxygen; Relaxation (psychology); Atomic electron transition; Spectral line; Quantum mechanics","score_opus":0.006551496922032575,"score_gpt":0.23146140983393293,"score_spread":0.22490991291190035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973559081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98110586,0.0002400075,0.012780043,0.00012579157,0.000022668464,0.00001712534,0.00022393871,0.00014376278,0.0053408225],"genre_scores_gemma":[0.9984012,0.000089983565,0.000950178,0.000014545341,0.0000031141037,0.0000089786445,0.00010051861,0.000022252112,0.00040919354],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999292,0.000010816239,0.0000027068825,0.000015354864,0.000020910617,0.000021005553],"domain_scores_gemma":[0.9996865,0.0001725357,0.00006870749,0.00002756291,0.000022335455,0.000022417187],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021561056,0.00026248046,0.00013382098,0.00034935414,0.00024755058,0.00021735617,0.0004456515,0.00032499866,0.0023559064],"category_scores_gemma":[0.00089992094,0.00019341556,0.0002900563,0.00024517163,0.00049877475,0.0003969642,0.00033094466,0.00039813525,0.00018444782],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012979201,0.0002303981,0.026508383,0.000609089,0.00010426775,0.0016103052,0.0011163804,0.27734402,0.57611406,0.07866742,0.0020211781,0.034376625],"study_design_scores_gemma":[0.00013789482,0.00025044006,0.051740263,0.00003263021,0.000043765976,0.00097112544,0.00035706905,0.6231005,0.29418975,0.026432479,0.0026518614,0.00009217103],"about_ca_topic_score_codex":0.0008236258,"about_ca_topic_score_gemma":0.00059487583,"teacher_disagreement_score":0.0023559064,"about_ca_system_score_codex":0.00043095415,"about_ca_system_score_gemma":0.00014078841,"threshold_uncertainty_score":0.007881284},"labels":[],"label_agreement":null},{"id":"W1973687676","doi":"10.1086/506171","title":"Accretion Disks around Young Stars: Lifetimes, Disk Locking, and Variability","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Accretion (finance); Planet; Stars; Accretion disc; Spectral line; Brown dwarf; Planetary system; Gas giant; Debris disk","score_opus":0.006434136965865717,"score_gpt":0.22625633480590973,"score_spread":0.219822197840044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973687676","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987608,0.00048926903,0.00022650092,0.000007516595,9.415769e-7,0.0000020621412,0.00018389335,0.000006113816,0.0003229082],"genre_scores_gemma":[0.9990175,0.000215154,0.00024290699,0.000006745351,0.0000054019492,0.0000029756675,0.00031878648,0.0000036143915,0.00018698946],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998934,0.000012816709,0.000011220952,0.000039351493,0.000023129778,0.000020100617],"domain_scores_gemma":[0.9987437,0.00027021012,0.0005924584,0.000103639584,0.00013948532,0.00015053793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041150805,0.0001290327,0.00019723184,0.0011245346,0.00038911874,0.00072838075,0.00027652227,0.000155639,0.0005938081],"category_scores_gemma":[0.0016699575,0.00011365671,0.00013508934,0.0010157214,0.00023697867,0.00053532363,0.0004840135,0.00020204255,0.0002497761],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059987473,0.00001848281,0.98189986,0.000021048969,0.000021810785,0.000076361175,0.00046688516,0.00013350675,0.007818971,0.000051637526,0.00004018165,0.009391273],"study_design_scores_gemma":[0.0000013611535,0.000032960783,0.99823004,0.0000041750122,0.000012605691,0.00028871818,0.00011855403,0.00018697132,0.0007086345,0.000071997165,0.00034114282,0.0000029513908],"about_ca_topic_score_codex":0.0019726034,"about_ca_topic_score_gemma":0.0028776461,"teacher_disagreement_score":0.0019726034,"about_ca_system_score_codex":0.0002125223,"about_ca_system_score_gemma":0.00013310475,"threshold_uncertainty_score":0.0039222836},"labels":[],"label_agreement":null},{"id":"W1973820299","doi":"10.1086/317785","title":"Efficiencies of Low‐Mass Star and Star Cluster Formation","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":389,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Stars; Physics; Star formation; Flattening; Star (game theory); Cluster (spacecraft); Initial mass function; Star cluster; Astronomy","score_opus":0.006548451326532607,"score_gpt":0.21393635264864683,"score_spread":0.2073879013221142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973820299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97255266,0.0001862162,0.01958209,0.00005182995,0.0000042029196,0.000014004359,0.00017337853,0.00017948315,0.0072561884],"genre_scores_gemma":[0.99801886,0.00005910184,0.0011162164,0.0000045674387,0.0000012287094,0.0000059342124,0.00009566735,0.000016586566,0.0006819553],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9996704,0.000051487863,0.000012866824,0.00007546078,0.000081674785,0.00010816704],"domain_scores_gemma":[0.9990251,0.00042139494,0.00019213308,0.00014497752,0.0001154327,0.00010105292],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005271163,0.00029350573,0.0002546908,0.0007321377,0.00023264955,0.0010081087,0.0006807694,0.00050030893,0.0014123949],"category_scores_gemma":[0.0029148532,0.00024184813,0.00050848065,0.0004707672,0.0006496704,0.0006199001,0.0005398068,0.00023693891,0.0006249165],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017860104,0.000057971218,0.1475368,0.000084980966,0.00007410164,0.00027196837,0.00022707711,0.7779485,0.022407692,0.030999558,0.00057877833,0.01963383],"study_design_scores_gemma":[0.000029167635,0.00010089418,0.08042216,0.000020661797,0.000035855835,0.0006990186,0.00012258878,0.87270457,0.03218983,0.01114495,0.002481959,0.00004843011],"about_ca_topic_score_codex":0.004975773,"about_ca_topic_score_gemma":0.002002303,"teacher_disagreement_score":0.004975773,"about_ca_system_score_codex":0.001205704,"about_ca_system_score_gemma":0.0004855352,"threshold_uncertainty_score":0.009893596},"labels":[],"label_agreement":null},{"id":"W1973860917","doi":"10.1086/432785","title":"M31’s Heavy‐Element Distribution and Outer Disk","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of British Columbia","funders":"","keywords":"Milky Way; Globular cluster; Stars; Halo; Brightness; Surface brightness; Scaling; RADIUS; Stellar evolution","score_opus":0.008263844244508812,"score_gpt":0.22320580673194435,"score_spread":0.21494196248743552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1973860917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977506,0.000032641317,0.00013027186,0.000020768495,5.059468e-7,0.000002876859,0.0004416132,0.0000111468835,0.0016096326],"genre_scores_gemma":[0.99810505,0.000024394221,0.00022889921,0.0000064170167,0.0000016993059,0.0000027099857,0.0009717061,0.0000028902857,0.0006561641],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999471,0.0000042533197,0.000002517155,0.00001665369,0.000010091797,0.000019359322],"domain_scores_gemma":[0.99970144,0.00004878315,0.00007182328,0.000036809517,0.00006859918,0.00007242381],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111346235,0.000114949384,0.00007633062,0.00084218,0.00030162086,0.00029949666,0.00013475215,0.00014130272,0.0022420594],"category_scores_gemma":[0.0003725716,0.00007482061,0.000088953,0.00058591145,0.00013996186,0.00021043012,0.00021409261,0.0000906058,0.00064564095],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036245806,0.0000643317,0.9107604,0.00002404384,0.000032963882,0.00038532933,0.00067694124,0.0025139833,0.048398793,0.0016036154,0.0031459997,0.032031104],"study_design_scores_gemma":[0.0000024329343,0.000018635044,0.9966869,0.0000020241184,0.0000017158347,0.00014766165,0.00006128707,0.0011435496,0.00069257506,0.00010300504,0.0011375987,0.000002554746],"about_ca_topic_score_codex":0.009201116,"about_ca_topic_score_gemma":0.006833039,"teacher_disagreement_score":0.009201116,"about_ca_system_score_codex":0.00043347134,"about_ca_system_score_gemma":0.0001377388,"threshold_uncertainty_score":0.01829511},"labels":[],"label_agreement":null},{"id":"W1974226132","doi":"10.1088/0004-637x/729/1/23","title":"A DEEP PHOTOMETRIC LOOK AT TWO OF ANDROMEDA'S DWARF SPHEROIDALS: X AND XVII","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"Science and Technology Facilities Council","keywords":"Andromeda; Red-giant branch; Physics; Astrophysics; Photometry (optics); Local Group; Galaxy; Metallicity; Dwarf galaxy; Astronomy; Horizontal branch; Globular cluster; Dwarf spheroidal galaxy; Milky Way; Stars; Interacting galaxy","score_opus":0.012070856688420476,"score_gpt":0.2164456701687824,"score_spread":0.20437481348036193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974226132","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99475265,0.00019733081,0.00047971262,0.0000317144,0.000004179003,0.000009111753,0.00041076023,0.00004851704,0.0040661017],"genre_scores_gemma":[0.99638355,0.00008326936,0.0014116083,0.000025251302,0.000008379996,0.000003619247,0.0009051731,0.000011177683,0.001167908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992394,0.0000071300697,0.0000025896181,0.000027326383,0.000017594328,0.000021288508],"domain_scores_gemma":[0.999788,0.000016061953,0.000067407265,0.00002522477,0.000018024804,0.00008523654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009524083,0.00024523571,0.00018270426,0.0007500019,0.00040054234,0.00037003262,0.00017955658,0.00017256827,0.00096901035],"category_scores_gemma":[0.00015413908,0.0001307824,0.0001681864,0.00047846755,0.00018305668,0.00016296032,0.0004555601,0.00029842128,0.00043927119],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019565447,0.00010334955,0.8638697,0.00007156943,0.0001078206,0.0006421273,0.00198294,0.00094484276,0.0948086,0.0010276119,0.0013350182,0.03491072],"study_design_scores_gemma":[0.0000046678933,0.000057484143,0.99498725,0.000003950859,0.000009627475,0.00028570776,0.00026379785,0.00029585775,0.0010195058,0.00006659469,0.0030002098,0.000005422163],"about_ca_topic_score_codex":0.0064876606,"about_ca_topic_score_gemma":0.0148149775,"teacher_disagreement_score":0.0064876606,"about_ca_system_score_codex":0.00022976683,"about_ca_system_score_gemma":0.00014518778,"threshold_uncertainty_score":0.012899816},"labels":[],"label_agreement":null},{"id":"W1974241900","doi":"10.1088/0004-637x/716/2/1345","title":"LONG-TERM X-RAY CHANGES IN THE EMISSION FROM THE ANOMALOUS X-RAY PULSAR 4U 0142+61","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Pulsar; Black-body radiation; Flux (metallurgy); Telescope; X-ray; Neutron star; X-ray pulsar; Light curve; Pulse (music); Astronomy; Optics; Radiation; Detector","score_opus":0.012996235656959104,"score_gpt":0.24195448942566586,"score_spread":0.22895825376870677,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974241900","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994467,0.00006377775,0.000032795517,0.000008483531,0.0000017124042,0.0000018443162,0.00009563799,0.0000045812117,0.0003445546],"genre_scores_gemma":[0.99883026,0.00007897109,0.00014278096,0.000012863272,0.000009917941,0.000007185886,0.0006741206,0.0000041466733,0.00023981079],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998629,0.000013649016,0.000011196633,0.000039557086,0.000039639257,0.000032984524],"domain_scores_gemma":[0.99947375,0.00008929998,0.00022253372,0.0000466557,0.000082858714,0.00008491082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022596311,0.00026319164,0.00025901003,0.00076593645,0.0003228087,0.0006124107,0.00018011626,0.0003759307,0.0005886733],"category_scores_gemma":[0.0008069175,0.00016321489,0.00022321175,0.0006406618,0.00026677683,0.0003096868,0.0006331441,0.00036570855,0.00018349689],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026015087,0.000107942345,0.9285747,0.000080928236,0.00013462317,0.0010668137,0.0004723502,0.00088941806,0.056987435,0.00010028705,0.00025205623,0.011073443],"study_design_scores_gemma":[0.0000020551672,0.000052517706,0.9984434,0.0000032080584,0.000009972169,0.00021388852,0.000056288067,0.00024029883,0.0006971148,0.000013293191,0.00026487806,0.0000031472782],"about_ca_topic_score_codex":0.0011360727,"about_ca_topic_score_gemma":0.0023847101,"teacher_disagreement_score":0.0011360727,"about_ca_system_score_codex":0.00018166372,"about_ca_system_score_gemma":0.00010459224,"threshold_uncertainty_score":0.0022588968},"labels":[],"label_agreement":null},{"id":"W1974279624","doi":"10.1086/587031","title":"The Infrared Detection of the Pulsar Wind Nebula in the Galactic Supernova Remnant 3C 58","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Supernova remnant; Pulsar; Pulsar wind nebula; Infrared; Nebula; Infrared astronomy; Emission nebula","score_opus":0.013806094831528998,"score_gpt":0.28094023553825637,"score_spread":0.26713414070672736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974279624","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98499197,0.00049323245,0.00047854625,0.00022618812,0.000047561916,0.000017745777,0.0001351908,0.00003483735,0.013574705],"genre_scores_gemma":[0.9959395,0.00019542307,0.0003795776,0.00018496602,0.000036305068,0.000009557776,0.00017314366,0.000011242025,0.003070333],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999378,0.000003914589,0.0000022291238,0.000021216687,0.000017196191,0.000017647488],"domain_scores_gemma":[0.99985576,0.000035499124,0.000023806066,0.000014760787,0.000025658243,0.000044555993],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003474041,0.0002707258,0.0002470804,0.00068487297,0.00063709344,0.00053522445,0.00032982777,0.00061843864,0.004656374],"category_scores_gemma":[0.00036750248,0.00019256909,0.00019850532,0.00021905512,0.00041094923,0.00024680517,0.0007809529,0.00054770237,0.00079075765],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014435758,0.00020921248,0.22759709,0.0001900695,0.00020938572,0.0071047773,0.0006334901,0.00043665487,0.72820497,0.0023267635,0.0028125502,0.028831528],"study_design_scores_gemma":[0.00014592429,0.0007815135,0.9472838,0.000058304155,0.00022218144,0.006117768,0.0004247154,0.0009145885,0.03210012,0.0010817582,0.010843532,0.000025849695],"about_ca_topic_score_codex":0.0016903066,"about_ca_topic_score_gemma":0.002058912,"teacher_disagreement_score":0.004656374,"about_ca_system_score_codex":0.00021202904,"about_ca_system_score_gemma":0.00013213267,"threshold_uncertainty_score":0.0155771375},"labels":[],"label_agreement":null},{"id":"W1974302678","doi":"10.1086/309201","title":"Five Years of Pulsar Flux Density Monitoring: Refractive Scintillation and the Interstellar Medium","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Vela; Interstellar medium; Scintillation; Neutron star; Flux (metallurgy); Line-of-sight; Stars; Astronomy; Galaxy; Optics","score_opus":0.00872667281705986,"score_gpt":0.29300521309162986,"score_spread":0.28427854027457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974302678","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99753773,0.00044935723,0.0008667649,0.000050527244,0.00001927161,0.000011933901,0.0003900723,0.000036421497,0.0006379255],"genre_scores_gemma":[0.9982481,0.00012255857,0.0004676098,0.00003430319,0.000022088047,0.00000805183,0.000841182,0.0000039852034,0.0002522153],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995915,0.00005736394,0.000055156837,0.00009164651,0.00011886141,0.00008548197],"domain_scores_gemma":[0.998538,0.00030717204,0.0004435515,0.00014459608,0.000331021,0.0002356365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009647282,0.0002088339,0.00036318888,0.0012843913,0.000602755,0.0006047509,0.00029794284,0.0004532948,0.00042561005],"category_scores_gemma":[0.0018032128,0.000110288376,0.000211495,0.00090695365,0.00025522607,0.00045250193,0.00067553023,0.00039006487,0.00009805395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035672015,0.0001886068,0.9514022,0.000059031205,0.00017003881,0.00038022595,0.00043400415,0.0013888166,0.014769157,0.00016365375,0.00038307838,0.03030437],"study_design_scores_gemma":[0.000008582101,0.0005936694,0.98998624,0.000016519258,0.00008635454,0.00035365604,0.00019707778,0.0018965723,0.0041376934,0.00012850271,0.0025744145,0.000020757765],"about_ca_topic_score_codex":0.004064901,"about_ca_topic_score_gemma":0.0065978398,"teacher_disagreement_score":0.004064901,"about_ca_system_score_codex":0.00030223455,"about_ca_system_score_gemma":0.00017065379,"threshold_uncertainty_score":0.008082449},"labels":[],"label_agreement":null},{"id":"W1974493970","doi":"10.1086/513066","title":"Evolution of Brown Dwarf Disks: A<i>Spitzer</i>Survey in Upper Scorpius","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Brown dwarf; Photometry (optics); Opacity; Stars; Circumstellar dust; Astronomy; Flux (metallurgy)","score_opus":0.013997798640402608,"score_gpt":0.2511133899372704,"score_spread":0.2371155912968678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974493970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918634,0.000036425477,0.000019639729,0.00000957573,5.7831375e-7,0.0000033364254,0.00021018705,0.000007154095,0.000526798],"genre_scores_gemma":[0.99790597,0.00008840356,0.00014952864,0.000017704924,0.0000035394185,0.000006380274,0.0009372487,0.0000067071305,0.00088442443],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998796,0.0000075138564,0.0000073525703,0.000037178856,0.00002489267,0.00004338788],"domain_scores_gemma":[0.9997044,0.000017119159,0.000091795686,0.000019286817,0.00005165261,0.000115728304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001442845,0.0002497011,0.00016882975,0.0016566726,0.0004576406,0.0004873786,0.0002303659,0.00014401905,0.0014410308],"category_scores_gemma":[0.00024061075,0.0001350229,0.00015133545,0.0007595392,0.0003595652,0.00020438993,0.000578032,0.000149265,0.00042884366],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037440415,0.000023646478,0.9892095,0.000014722225,0.000014064452,0.000319718,0.0007568959,0.000056637276,0.0046725604,0.000041782383,0.00023730395,0.0046156757],"study_design_scores_gemma":[5.638956e-7,0.000015227048,0.9990702,0.0000036484041,0.0000030280505,0.00010408786,0.00022282542,0.00002745994,0.00015469885,0.0000058750866,0.00039142751,9.148845e-7],"about_ca_topic_score_codex":0.032680172,"about_ca_topic_score_gemma":0.052029535,"teacher_disagreement_score":0.032680172,"about_ca_system_score_codex":0.00041934,"about_ca_system_score_gemma":0.00026459634,"threshold_uncertainty_score":0.06497991},"labels":[],"label_agreement":null},{"id":"W1974543936","doi":"10.1088/0004-637x/693/1/23","title":"ATMOSPHERIC ESCAPE FROM HOT JUPITERS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":717,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Hot Jupiter; Astrophysics; Planet; Atmospheric escape; T Tauri star; Astronomy; Stars; Exoplanet","score_opus":0.0073187867763024154,"score_gpt":0.20784589063554254,"score_spread":0.20052710385924014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974543936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9807931,0.0002573475,0.005501519,0.00021278654,0.000021074708,0.00002049386,0.0002065171,0.000186117,0.012801105],"genre_scores_gemma":[0.9971054,0.00011830431,0.00042633095,0.00004740879,0.000013190004,0.000013207111,0.0001412517,0.000018728691,0.0021161244],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995077,0.0000062741697,0.0000012118294,0.000013474882,0.000009151622,0.000019139838],"domain_scores_gemma":[0.9999398,0.00000756014,0.000016179369,0.000007989029,0.000004069345,0.00002434325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005956964,0.00047628404,0.00036541006,0.00011554754,0.0006408994,0.000628707,0.0005201515,0.00067986397,0.0019933253],"category_scores_gemma":[0.00020925626,0.00018402656,0.00057359773,0.00009842239,0.00040070064,0.00060807535,0.0008745856,0.00044170953,0.00024812456],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005793948,0.00026032142,0.07899599,0.00024851726,0.00021091549,0.0019367655,0.0009772538,0.76375717,0.0879188,0.04516781,0.0048832386,0.015063728],"study_design_scores_gemma":[0.0002582335,0.0006527363,0.047054894,0.00004396667,0.00007960894,0.00073925714,0.00034004645,0.9253702,0.0054973513,0.01274096,0.0071563,0.00006648215],"about_ca_topic_score_codex":0.0094976025,"about_ca_topic_score_gemma":0.004016427,"teacher_disagreement_score":0.0094976025,"about_ca_system_score_codex":0.0006619993,"about_ca_system_score_gemma":0.0002460132,"threshold_uncertainty_score":0.018884659},"labels":[],"label_agreement":null},{"id":"W1974567023","doi":"10.1086/525839","title":"Relativistic Effects in Extreme Mass Ratio Gravitational Wave Bursts","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph","funders":"","keywords":"Physics; Gravitational wave; Relativistic quantum chemistry; Black hole (networking); Astrophysics; Amplitude; Dephasing; Interferometry; Quantum mechanics","score_opus":0.03253807482952401,"score_gpt":0.2923961763531358,"score_spread":0.2598581015236118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974567023","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9516352,0.0020185742,0.038935635,0.00024266669,0.000119698736,0.000019345496,0.00007269004,0.0003676198,0.006588534],"genre_scores_gemma":[0.99765295,0.0003020562,0.0014816049,0.000031765067,0.000059715625,0.0000032111054,0.00004813368,0.00004634718,0.00037411085],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99978524,0.00008400155,0.000012571455,0.00003436381,0.000043274864,0.000040599192],"domain_scores_gemma":[0.99781585,0.0010145478,0.0006918321,0.00025500072,0.00011694675,0.000105812716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061959535,0.0004451618,0.00031674205,0.0006126611,0.0002646415,0.000510756,0.0005900414,0.00048527188,0.0011686004],"category_scores_gemma":[0.0044645085,0.00022775127,0.00039109177,0.00049796194,0.0005022467,0.0005942106,0.00060370157,0.00040910312,0.00016922446],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018259583,0.00025905683,0.25870332,0.0007680916,0.00043291712,0.007131182,0.0016960118,0.2947674,0.17084289,0.16690333,0.0031170773,0.09355267],"study_design_scores_gemma":[0.00021738421,0.0007191554,0.2986184,0.00010542744,0.00034483118,0.003921542,0.00032341134,0.6017684,0.022802277,0.061879363,0.009070378,0.0002295345],"about_ca_topic_score_codex":0.0006475393,"about_ca_topic_score_gemma":0.00038305126,"teacher_disagreement_score":0.0011686004,"about_ca_system_score_codex":0.00024509124,"about_ca_system_score_gemma":0.000107717075,"threshold_uncertainty_score":0.003909409},"labels":[],"label_agreement":null},{"id":"W1974594065","doi":"10.1088/0004-637x/738/2/158","title":"EXTENDED SUBMILLIMETER EMISSION OF THE GALACTIC CENTER AND NEAR-INFRARED/SUBMILLIMETER VARIABILITY OF ITS SUPERMASSIVE BLACK HOLE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galactic Center; Supermassive black hole; Spectral index; Galaxy; Molecular cloud; Astronomy; Submillimeter Array; Radiative transfer; Active galactic nucleus; Black hole (networking); Infrared; Flux (metallurgy); Sagittarius A*; Star formation; Spectral line; Stars","score_opus":0.01808125330368566,"score_gpt":0.22416530769489773,"score_spread":0.20608405439121208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974594065","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982387,0.00013820826,0.00011861443,0.000011909121,0.000001929644,0.0000021772157,0.00035758267,0.000026946745,0.0011039198],"genre_scores_gemma":[0.9989774,0.00006999091,0.0001856575,0.000010844296,0.0000066515104,0.0000024585538,0.0005363252,0.0000057829184,0.00020479353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997723,0.0000015889002,7.997527e-7,0.000009337781,0.0000045067914,0.0000064277165],"domain_scores_gemma":[0.99992526,0.0000070778797,0.000030677485,0.000005871171,0.000009432921,0.000021695541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006370126,0.00017717811,0.00010978492,0.00037021996,0.00009812251,0.00024574573,0.00013267568,0.00009190323,0.0009449602],"category_scores_gemma":[0.000094389776,0.00007683862,0.000101653575,0.00028604353,0.00008970944,0.0001262613,0.00015579164,0.000102004495,0.00024721754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013856044,0.000051870302,0.8993604,0.000038852024,0.00010460038,0.00020090428,0.00024686352,0.000587984,0.080911465,0.0003165799,0.0010051519,0.017036706],"study_design_scores_gemma":[0.0000011646664,0.00000723052,0.9993067,0.0000011198224,0.000006058982,0.00004205097,0.000015106521,0.00014854874,0.00026256105,0.000013812982,0.00019500552,6.4279254e-7],"about_ca_topic_score_codex":0.003860458,"about_ca_topic_score_gemma":0.0045883306,"teacher_disagreement_score":0.003860458,"about_ca_system_score_codex":0.00011829626,"about_ca_system_score_gemma":0.00003805053,"threshold_uncertainty_score":0.0076759458},"labels":[],"label_agreement":null},{"id":"W1974653568","doi":"10.1086/497952","title":"Oxygen from the λ7774 High‐Excitation Triplet in Open Cluster Dwarfs: Hyades","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Pleiades; Physics; Open cluster; Starspot; Stars; Effective temperature; Stellar classification; Abundance (ecology); Spectral line; Star cluster; Astronomy; Biology; Ecology","score_opus":0.015658292116077194,"score_gpt":0.2467791859354379,"score_spread":0.2311208938193607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974653568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99944335,0.00003571821,0.000024655214,0.000009058087,0.0000015795544,0.0000010781264,0.00016689513,0.000002935174,0.00031463648],"genre_scores_gemma":[0.99871075,0.000041004358,0.00007025239,0.000010517481,0.0000055578316,0.0000024164908,0.00074313907,0.000005073278,0.00041119193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.0000045887246,0.0000025201632,0.000021953465,0.000014415404,0.000019538278],"domain_scores_gemma":[0.99981445,0.000014322435,0.00005481587,0.000016610893,0.00003263885,0.000067123714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010579445,0.00024957873,0.0002792759,0.0007643415,0.00067199377,0.00048176912,0.00028750984,0.00029813862,0.0011013693],"category_scores_gemma":[0.00016453762,0.00016438942,0.00010204293,0.0006430231,0.00031690457,0.0002830272,0.00032325124,0.00022583603,0.00024158401],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011087822,0.00018472472,0.87952816,0.00004017996,0.000093342474,0.00031336443,0.0005952436,0.0006989005,0.10981294,0.00048749772,0.00080734317,0.0063295076],"study_design_scores_gemma":[0.000010515663,0.00003976408,0.99692625,0.0000029800742,0.000022628905,0.00009643105,0.00017587052,0.00040755054,0.0017565999,0.00007603513,0.0004821815,0.000003209749],"about_ca_topic_score_codex":0.023336621,"about_ca_topic_score_gemma":0.043551598,"teacher_disagreement_score":0.023336621,"about_ca_system_score_codex":0.00061491545,"about_ca_system_score_gemma":0.00016405525,"threshold_uncertainty_score":0.04640156},"labels":[],"label_agreement":null},{"id":"W1974668797","doi":"10.1086/344608","title":"The Canada–United Kingdom Deep Submillimeter Survey. V. The Submillimeter Properties of Lyman Break Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Galaxy; Redshift; Physics; Flux (metallurgy); Sample (material); Amplitude; Astronomy; Submillimeter Array; Star formation; Materials science; Optics","score_opus":0.016659771225001143,"score_gpt":0.2006558834353775,"score_spread":0.18399611221037634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974668797","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.070897356,0.0046867263,0.0014769776,0.0026628554,0.00036043057,0.000245308,0.84483624,0.0005910144,0.07424316],"genre_scores_gemma":[0.33956608,0.003966494,0.009731155,0.0019182204,0.0001556108,0.00045129776,0.47584435,0.00041323717,0.1679535],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9992592,0.000041298998,0.00003411415,0.00010886669,0.0003291709,0.00022746077],"domain_scores_gemma":[0.99683565,0.00009442178,0.0004039741,0.0001804917,0.0020405406,0.0004448825],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052946183,0.00055197865,0.00046511486,0.0035552902,0.0011510936,0.0011977843,0.00094329834,0.0004374401,0.017149135],"category_scores_gemma":[0.0014668949,0.00028091314,0.0003650107,0.0055096056,0.00034609454,0.00051894266,0.000885046,0.0006608111,0.004522623],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021526487,0.000059162117,0.25586444,0.00041280963,0.00016335948,0.00018993289,0.00049681,0.0005737116,0.0018255081,0.0034804202,0.68147296,0.055245545],"study_design_scores_gemma":[0.000028394237,0.000012580643,0.74510676,0.00009209363,0.000022458818,0.00006762556,0.00029118278,0.00028264394,0.0005058319,0.00016721564,0.25339776,0.000025483518],"about_ca_topic_score_codex":0.9680445,"about_ca_topic_score_gemma":0.97979194,"teacher_disagreement_score":0.03195548,"about_ca_system_score_codex":0.012453529,"about_ca_system_score_gemma":0.012114033,"threshold_uncertainty_score":0.090357065},"labels":[],"label_agreement":null},{"id":"W1974798231","doi":"10.1086/338576","title":"Gravity and Nongravity Modes in the VIRMOS‐DESCART Weak‐Lensing Survey","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Weak gravitational lensing; Observable; Gravitational lens; Dark matter; Spectral density; Mode (computer interface); Noise (video); SIGNAL (programming language); Astrophysics; Statistical physics; Galaxy; Statistics; Quantum mechanics; Image (mathematics)","score_opus":0.016954203130915266,"score_gpt":0.22093344134099088,"score_spread":0.20397923821007563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974798231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99908364,0.00002159314,0.00010527245,0.000016644484,5.594711e-7,8.5661827e-7,0.0004118,0.000006557503,0.0003531144],"genre_scores_gemma":[0.9985557,0.000033760487,0.00011929145,0.000005483352,0.0000030391104,0.0000018180095,0.0011053488,0.0000043794,0.00017102905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998272,0.000038634316,0.000012539713,0.000039903378,0.000042238873,0.00003958805],"domain_scores_gemma":[0.9991129,0.00017437286,0.00034019322,0.00009317143,0.00009650285,0.00018286514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003040481,0.0002332261,0.00016262813,0.001991995,0.00025391227,0.0006467914,0.00021039041,0.000158369,0.0008214603],"category_scores_gemma":[0.0014911224,0.00013131773,0.00016449604,0.001711362,0.00046744363,0.0002750236,0.000532018,0.00014884387,0.00026805646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000117314004,0.000018144761,0.98790014,0.000008322138,0.000039209244,0.00006376038,0.0002840799,0.0014859227,0.0029427307,0.0014466128,0.0004652669,0.005228446],"study_design_scores_gemma":[0.0000027688468,0.00000860498,0.99731284,0.0000016777832,0.0000060396424,0.000028650951,0.00007412515,0.0016890366,0.00028816366,0.0002493749,0.00033325428,0.0000054266893],"about_ca_topic_score_codex":0.022911271,"about_ca_topic_score_gemma":0.026793139,"teacher_disagreement_score":0.022911271,"about_ca_system_score_codex":0.00037928368,"about_ca_system_score_gemma":0.00022280645,"threshold_uncertainty_score":0.04555583},"labels":[],"label_agreement":null},{"id":"W1974823915","doi":"10.1088/0004-637x/697/1/900","title":"STELLAR-MASS BLACK HOLE SPIN CONSTRAINTS FROM DISK REFLECTION AND CONTINUUM MODELING","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":256,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Black hole (networking); Spin-flip; Stellar black hole; Intermediate-mass black hole; Astrophysics; Binary black hole; Rotating black hole; Supermassive black hole; Accretion (finance); Astronomy; Gravitational wave; Galaxy","score_opus":0.017866324368675968,"score_gpt":0.2542593708133302,"score_spread":0.23639304644465425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974823915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994532,0.000073151685,0.004434751,0.000027357684,0.0000016907763,0.000005527899,0.000052422136,0.000028074004,0.0008451243],"genre_scores_gemma":[0.99861157,0.000035663335,0.0011953713,0.000004589842,0.0000037323725,0.0000022926536,0.00008269484,0.000008139316,0.000055997738],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996555,0.00012747337,0.000028317892,0.000057618952,0.000067417364,0.000063593],"domain_scores_gemma":[0.9973869,0.0012551128,0.00053788023,0.00042094392,0.00020612025,0.00019302953],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014265507,0.0007004845,0.0006015492,0.0008104881,0.00042698806,0.0014457447,0.0005732354,0.00034170298,0.0011589393],"category_scores_gemma":[0.005748112,0.000284573,0.00058834907,0.00042402095,0.00042120452,0.0006536028,0.00081517565,0.00033357725,0.00023065646],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010403697,0.00015119696,0.79750323,0.0001183271,0.00025439958,0.0005010776,0.0005002893,0.13447514,0.026684878,0.009018969,0.00041621918,0.029335989],"study_design_scores_gemma":[0.00013010768,0.00020246071,0.22290468,0.000041506184,0.00024743818,0.00032723296,0.00040690947,0.74967164,0.012615185,0.012471465,0.0009310037,0.000050345923],"about_ca_topic_score_codex":0.0017475263,"about_ca_topic_score_gemma":0.0019542575,"teacher_disagreement_score":0.0017475263,"about_ca_system_score_codex":0.0003243372,"about_ca_system_score_gemma":0.00028261708,"threshold_uncertainty_score":0.0075443983},"labels":[],"label_agreement":null},{"id":"W1974885844","doi":"10.1088/0004-637x/728/2/100","title":"THE BLACK HOLE MASS IN THE BRIGHTEST CLUSTER GALAXY NGC 6086","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; University of Texas at Austin; W. M. Keck Foundation; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Dark matter; Astronomy; Stellar mass; Dark matter halo; Black hole (networking); Star cluster; Solar mass; Observatory; Galaxy cluster; Halo; Star formation","score_opus":0.011067104674761581,"score_gpt":0.20663602854611615,"score_spread":0.19556892387135458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974885844","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951506,0.00005111911,0.00009264989,0.0000065994473,8.2078935e-7,7.2970647e-7,0.000054874086,0.000011764798,0.00026642522],"genre_scores_gemma":[0.99965096,0.000023146564,0.00011870931,0.000004241946,0.0000019795425,4.661082e-7,0.00011770398,0.000002019812,0.00008062981],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988675,0.000010309127,0.0000064535952,0.00004353554,0.000026193953,0.000026780905],"domain_scores_gemma":[0.9996731,0.000036509286,0.00012273775,0.000038039245,0.000034385917,0.00009518998],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018734478,0.00022500256,0.00025872176,0.000716287,0.0004059989,0.0004557892,0.00023905489,0.00024472302,0.0005029337],"category_scores_gemma":[0.0005842588,0.000132802,0.00012806251,0.00041088066,0.0003877213,0.00024327693,0.00044762253,0.00013289523,0.0002665132],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001512723,0.00002385554,0.9759473,0.000014098117,0.000025741376,0.00010286314,0.00027294582,0.000959244,0.015694603,0.00018729654,0.00020155266,0.0064192396],"study_design_scores_gemma":[0.000004300886,0.000027351743,0.9974492,0.0000025097995,0.000008574388,0.00008604134,0.000041647327,0.0012234219,0.00088480144,0.000057578094,0.00021142434,0.0000030674435],"about_ca_topic_score_codex":0.009892654,"about_ca_topic_score_gemma":0.0127937645,"teacher_disagreement_score":0.009892654,"about_ca_system_score_codex":0.00037411452,"about_ca_system_score_gemma":0.00009118323,"threshold_uncertainty_score":0.019670129},"labels":[],"label_agreement":null},{"id":"W1974968648","doi":"10.1086/508704","title":"Polarization of Absorption Lines as a Diagnostics of Circumstellar, Interstellar, and Intergalactic Magnetic Fields: Fine‐Structure Atoms","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Radiative transfer; Polarization (electrochemistry); Intergalactic travel; Anisotropy; Magnetic field; Linear polarization; Interstellar medium; Degenerate energy levels; Population; Absorption (acoustics); Atomic physics; Computational physics; Astrophysics; Optics; Galaxy; Redshift; Quantum mechanics","score_opus":0.0027442516582675135,"score_gpt":0.19292110259860462,"score_spread":0.1901768509403371,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974968648","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9749707,0.00013840813,0.022437355,0.000044343706,0.0000033309773,0.0000040573627,0.00007973795,0.00009750616,0.0022245166],"genre_scores_gemma":[0.9984987,0.000035777335,0.0013448418,0.0000031040918,0.0000018584267,0.0000017730762,0.000023787452,0.0000036483136,0.00008652301],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994683,0.000021880025,0.0000013387694,0.00000764823,0.000013723938,0.000008610552],"domain_scores_gemma":[0.99975127,0.0000994372,0.00007674046,0.00002808454,0.000025195644,0.000019278195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016264022,0.00015224729,0.00006361385,0.0004732862,0.00013480162,0.00035401862,0.00014429977,0.00021321503,0.0005577966],"category_scores_gemma":[0.0006115813,0.00007780823,0.00008476738,0.00046170046,0.0003262659,0.00023818534,0.00018951527,0.00012326146,0.000092376904],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000517657,0.0001218274,0.40333146,0.00013806288,0.00010384765,0.0005738708,0.00044436823,0.061973855,0.43016803,0.027663462,0.0009092866,0.074054256],"study_design_scores_gemma":[0.000045618683,0.00013331803,0.47942212,0.000024584942,0.00005245443,0.001103002,0.00031641236,0.36121622,0.13407645,0.021195995,0.002364142,0.000049791895],"about_ca_topic_score_codex":0.0003310548,"about_ca_topic_score_gemma":0.00027393497,"teacher_disagreement_score":0.0005577966,"about_ca_system_score_codex":0.00010499215,"about_ca_system_score_gemma":0.00006914168,"threshold_uncertainty_score":0.0018660426},"labels":[],"label_agreement":null},{"id":"W1974990852","doi":"10.1088/0004-637x/748/1/30","title":"A SUBSTELLAR COMPANION TO THE DUSTY PLEIADES STAR HD 23514","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Pleiades; Brown dwarf; Stars; Star (game theory); A-type main-sequence star; Adaptive optics; Main sequence","score_opus":0.020685239351292392,"score_gpt":0.27840522174122895,"score_spread":0.25771998238993654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1974990852","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978276,0.00013060847,0.0003326843,0.00006261818,0.000020399664,0.000006115862,0.00014509278,0.000024906769,0.0014499858],"genre_scores_gemma":[0.99560237,0.00008670954,0.0014682886,0.00004826508,0.000015037338,0.000004125015,0.0005074863,0.000004991783,0.0022626729],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999902,0.000006172822,0.0000066643115,0.00003248848,0.00003303435,0.000019578873],"domain_scores_gemma":[0.9996768,0.000040394745,0.000073801704,0.000041596766,0.000030393194,0.00013704467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001682748,0.00017977705,0.00020775945,0.00042307068,0.00092295243,0.0005376099,0.00035818765,0.000308135,0.002483773],"category_scores_gemma":[0.0003575926,0.00019572022,0.00012872413,0.00028153707,0.000290744,0.00036377646,0.0006415787,0.00035826495,0.0004893769],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042721105,0.00032440646,0.7834341,0.00012088439,0.00009710435,0.010107617,0.001478509,0.00050180935,0.16774005,0.0016653014,0.0021298106,0.0319732],"study_design_scores_gemma":[0.00004137505,0.000925775,0.92543393,0.000018449779,0.00006022756,0.015242873,0.0008063721,0.0017859855,0.026192058,0.00053989264,0.02891885,0.000034287943],"about_ca_topic_score_codex":0.002977707,"about_ca_topic_score_gemma":0.0049285754,"teacher_disagreement_score":0.002977707,"about_ca_system_score_codex":0.00026862495,"about_ca_system_score_gemma":0.00031646405,"threshold_uncertainty_score":0.008309066},"labels":[],"label_agreement":null},{"id":"W1975041259","doi":"10.1086/509103","title":"Light Curves for Rapidly Rotating Neutron Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; University of Alberta","funders":"","keywords":"Neutron star; Physics; Pulsar; RADIUS; Rotation (mathematics); Stellar rotation; Light curve; Star (game theory); Astrophysics; X-ray binary; Ray tracing (physics); Stars; Optics; Geometry","score_opus":0.010328985686611046,"score_gpt":0.3005041217906522,"score_spread":0.29017513610404116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975041259","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97979444,0.00017152113,0.013511726,0.00008833522,0.000017564766,0.00002255752,0.00022429274,0.00025264802,0.0059170304],"genre_scores_gemma":[0.9909299,0.00019394839,0.007112601,0.000018970642,0.000011523385,0.000015513895,0.00058465335,0.00015971082,0.00097311544],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981815,0.000050317172,0.000009608183,0.000024734678,0.00005431118,0.000042807605],"domain_scores_gemma":[0.9990395,0.00029634082,0.0001399644,0.00007582523,0.00029995042,0.00014840085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057370495,0.0004913468,0.0005333864,0.0011786703,0.0007423292,0.0008834006,0.00058508496,0.00054464577,0.0015609026],"category_scores_gemma":[0.0026423088,0.00024957565,0.0008525159,0.0011816877,0.00049456314,0.00051093975,0.00071394333,0.00081763975,0.0004505412],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041693868,0.00008730521,0.033928815,0.00008695273,0.0000807841,0.0007625248,0.0007168082,0.8934911,0.03307905,0.025259446,0.0008080775,0.011282237],"study_design_scores_gemma":[0.00007878765,0.00015240356,0.0155351525,0.000025125695,0.000022911092,0.00030144985,0.0002356298,0.96378773,0.01073049,0.0070265275,0.0020543395,0.000049438713],"about_ca_topic_score_codex":0.005326839,"about_ca_topic_score_gemma":0.0025248504,"teacher_disagreement_score":0.005326839,"about_ca_system_score_codex":0.0010963436,"about_ca_system_score_gemma":0.00040806548,"threshold_uncertainty_score":0.010591686},"labels":[],"label_agreement":null},{"id":"W1975080613","doi":"10.1088/0004-637x/724/2/1524","title":"STELLAR POPULATIONS OF Lyα EMITTERS AT<i>z</i>∼ 6-7: CONSTRAINTS ON THE ESCAPE FRACTION OF IONIZING PHOTONS FROM GALAXY BUILDING BLOCKS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":182,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Redshift; Galaxy; Extinction (optical mineralogy); Astronomy; Interstellar medium; Reionization; Stellar mass; Supernova; Star formation","score_opus":0.012310000931731116,"score_gpt":0.22698563465059995,"score_spread":0.21467563371886883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975080613","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999506,0.000034662477,0.00011972128,0.000003001663,3.2316652e-7,0.000001132933,0.00009091573,0.000004853264,0.00023938969],"genre_scores_gemma":[0.99936074,0.000025394522,0.00017821304,0.000004938828,0.0000017281222,0.0000015625868,0.00034973223,0.000002950583,0.00007453451],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998578,0.000013523358,0.000009385982,0.000046259956,0.000028231232,0.000044765595],"domain_scores_gemma":[0.9993044,0.00013166698,0.00027108006,0.000048325866,0.00008553047,0.00015888416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039773335,0.00029047084,0.00026638212,0.00078588683,0.00023024422,0.0006188213,0.0002974629,0.0003076659,0.0010631533],"category_scores_gemma":[0.00059655274,0.0002437041,0.0003249968,0.00031335285,0.00021451659,0.00044291012,0.00041180608,0.00019927413,0.00048088795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009194862,0.000019855343,0.9874024,0.0000075086473,0.000029737917,0.00002782486,0.00009192408,0.00026632161,0.010062104,0.000065403365,0.000030520456,0.0019044532],"study_design_scores_gemma":[0.000003619331,0.00003561834,0.9974058,0.000002558594,0.000018070321,0.00007370929,0.000079956444,0.000977232,0.001237515,0.000050623148,0.00011295858,0.000002366441],"about_ca_topic_score_codex":0.001662712,"about_ca_topic_score_gemma":0.0025329778,"teacher_disagreement_score":0.001662712,"about_ca_system_score_codex":0.0002132258,"about_ca_system_score_gemma":0.0000552382,"threshold_uncertainty_score":0.0035566688},"labels":[],"label_agreement":null},{"id":"W1975148044","doi":"10.1086/425960","title":"<i>Chandra</i>Spatially Resolved Spectroscopic Study and Multiwavelength Imaging of the Supernova Remnant 3C 397 (G41.1−0.3)","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Physics; Astrophysics; Supernova remnant; Ejecta; Pulsar; Pulsar wind nebula; Supernova; Nebula; Flux (metallurgy); Imaging spectrometer; Astronomy; Line-of-sight; Ionization; Spectrometer; Stars; Optics","score_opus":0.007123331579040857,"score_gpt":0.2212300605171091,"score_spread":0.21410672893806826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975148044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9735421,0.0012717868,0.00157786,0.0003752603,0.000099830104,0.00014283061,0.007952284,0.0005880141,0.014450159],"genre_scores_gemma":[0.97656566,0.00081333326,0.010344968,0.00025465066,0.00015283127,0.000055263157,0.008632432,0.00011444242,0.0030663614],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995434,0.0000016352775,0.0000029311768,0.000010782647,0.000014162456,0.000016103066],"domain_scores_gemma":[0.99980503,0.0000129529235,0.000055559813,0.000027048214,0.00003348524,0.000065909546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008347964,0.00023469524,0.00021504864,0.0016953746,0.0006222584,0.00031737745,0.00042911276,0.00028975614,0.003786846],"category_scores_gemma":[0.00013810178,0.00012210192,0.00026977554,0.0007874232,0.0002453751,0.00024490882,0.0003942889,0.0003695033,0.0005913506],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011095599,0.00036589892,0.22581513,0.00060365174,0.00021564496,0.018597389,0.0006941992,0.0018974305,0.6489705,0.0021199507,0.03282425,0.0667865],"study_design_scores_gemma":[0.00004050507,0.00022579441,0.92332065,0.000041808336,0.000054346543,0.014761347,0.00028718766,0.0012004983,0.023333386,0.00056211196,0.03612351,0.00004888412],"about_ca_topic_score_codex":0.0057635326,"about_ca_topic_score_gemma":0.012854414,"teacher_disagreement_score":0.0057635326,"about_ca_system_score_codex":0.00025559572,"about_ca_system_score_gemma":0.00018984172,"threshold_uncertainty_score":0.012668192},"labels":[],"label_agreement":null},{"id":"W1975197937","doi":"10.1086/377348","title":"<i>Chandra</i> Detection of a Pulsar Wind Nebula Associated with Supernova Remnant 3C 396","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Physics; Supernova remnant; Pulsar wind nebula; Pulsar; Astrophysics; Nebula; Astronomy; Emission nebula; Neutron star; Crab Nebula; Reflection nebula; Observatory; Supernova; Stars","score_opus":0.009815021207195861,"score_gpt":0.26479422134164243,"score_spread":0.2549792001344466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975197937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945115,0.00016961212,0.0002229069,0.000078445606,0.000013649027,0.00001748016,0.00140433,0.00012331216,0.0034587292],"genre_scores_gemma":[0.994173,0.00015286323,0.001649775,0.00007309613,0.00003985429,0.0000144234655,0.0028101832,0.000026748103,0.0010601309],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999081,0.0000043441514,0.0000055867317,0.000017902827,0.000040225274,0.000023885246],"domain_scores_gemma":[0.99970585,0.000015133684,0.000063188614,0.00003557473,0.00004230881,0.0001378961],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013957258,0.0002989632,0.00023553344,0.00089049904,0.0007468819,0.00047292904,0.00038230614,0.00039032448,0.0029653148],"category_scores_gemma":[0.00028445068,0.00013834125,0.00021356638,0.0006164132,0.00024798219,0.00017005668,0.0006147171,0.00032229238,0.00072672125],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019290582,0.00028538998,0.3384008,0.00029107486,0.0001718015,0.012323848,0.00072143716,0.000760709,0.60725504,0.0008379514,0.0070917546,0.029931169],"study_design_scores_gemma":[0.00005594468,0.00023786344,0.95697176,0.0000271114,0.000039119164,0.009465891,0.00013604423,0.0007702246,0.020764159,0.00021025013,0.0112911835,0.00003037184],"about_ca_topic_score_codex":0.006970232,"about_ca_topic_score_gemma":0.01583025,"teacher_disagreement_score":0.006970232,"about_ca_system_score_codex":0.00031485793,"about_ca_system_score_gemma":0.00017892882,"threshold_uncertainty_score":0.013859332},"labels":[],"label_agreement":null},{"id":"W1975212472","doi":"10.1088/0004-637x/706/1/571","title":"<i>K2</i>: A NEW METHOD FOR THE DETECTION OF GALAXY CLUSTERS BASED ON CANADA–FRANCE–HAWAII TELESCOPE LEGACY SURVEY MULTICOLOR IMAGES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Redshift; Astrophysics; Galaxy cluster; Cluster (spacecraft); Galaxy; Telescope; Photometric redshift; Astronomy; Computer science","score_opus":0.009151432891073584,"score_gpt":0.24192063111228732,"score_spread":0.23276919822121372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975212472","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1056057,0.00059215195,0.8329073,0.00040210076,0.00025383453,0.00041734774,0.009087768,0.03473932,0.015994448],"genre_scores_gemma":[0.28174183,0.00019780517,0.7027864,0.00025783444,0.000080249076,0.00026131282,0.005641362,0.0020400293,0.006993264],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992847,0.00007651222,0.000027234477,0.00019496199,0.00028014695,0.00013643835],"domain_scores_gemma":[0.9987729,0.00016710654,0.00020904481,0.00032875477,0.000394584,0.00012752356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008330303,0.00079760724,0.0005114241,0.002529797,0.0007634785,0.0012705481,0.0015236804,0.0004541832,0.0039341794],"category_scores_gemma":[0.0020233565,0.0005461203,0.000845336,0.0013194726,0.00051895133,0.0010358099,0.0012414851,0.0005815177,0.0020910038],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007676132,0.00016579748,0.1208169,0.00066661654,0.0008514845,0.00053213723,0.00061207864,0.04342368,0.14081043,0.01786117,0.06444182,0.6090503],"study_design_scores_gemma":[0.00017376723,0.00014995522,0.11180635,0.00007605857,0.00019614406,0.0011457972,0.0002256711,0.650117,0.14532734,0.00869386,0.08155585,0.0005321604],"about_ca_topic_score_codex":0.054954648,"about_ca_topic_score_gemma":0.08672459,"teacher_disagreement_score":0.054954648,"about_ca_system_score_codex":0.0015301986,"about_ca_system_score_gemma":0.0017107561,"threshold_uncertainty_score":0.10926956},"labels":[],"label_agreement":null},{"id":"W1975224492","doi":"10.1086/375263","title":"Shadowing-based Reliability Decay in Softened <i>n</i> -Body Simulations","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Scientific Research and Discoveries","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Softening; Exponential decay; Particle (ecology); Physics; Integrator; Particle number; Exponential function; Constant (computer programming); Mechanics; Classical mechanics; Mathematical analysis; Mathematics; Thermodynamics; Volume (thermodynamics); Computer science; Quantum mechanics","score_opus":0.012218940083168954,"score_gpt":0.27434993613452957,"score_spread":0.26213099605136064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975224492","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8696646,0.00042006586,0.1249055,0.00028053814,0.000047639955,0.00006375259,0.00015335367,0.000812274,0.0036522243],"genre_scores_gemma":[0.9867422,0.000069609414,0.012497074,0.000033414573,0.000004482954,0.00003181846,0.000098401106,0.0000797176,0.00044338836],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991567,0.0002417529,0.00004403025,0.00010356108,0.00029668325,0.00015724936],"domain_scores_gemma":[0.99303097,0.0041758646,0.00062541774,0.001053899,0.0007054309,0.00040843256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026806442,0.0004400675,0.000603136,0.0007872889,0.0004999774,0.0007208631,0.0014631532,0.000807102,0.001211881],"category_scores_gemma":[0.015411623,0.00041534548,0.0005259269,0.0003459212,0.0013214452,0.0011359033,0.0011150914,0.00120872,0.00016012661],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022585533,0.000055169367,0.008883033,0.00006506134,0.000041220916,0.00015126479,0.0002657693,0.968406,0.005484337,0.006019736,0.00038192264,0.010020592],"study_design_scores_gemma":[0.0000045083684,0.000017528371,0.00046793255,0.000007049279,0.0000033806043,0.000010754999,0.000010345073,0.9973085,0.0013229526,0.0007663645,0.00007507938,0.0000056782847],"about_ca_topic_score_codex":0.007813138,"about_ca_topic_score_gemma":0.005449541,"teacher_disagreement_score":0.007813138,"about_ca_system_score_codex":0.0014602516,"about_ca_system_score_gemma":0.0012389927,"threshold_uncertainty_score":0.015535295},"labels":[],"label_agreement":null},{"id":"W1975260087","doi":"10.1086/533428","title":"Accretion‐powered Stellar Winds. II. Numerical Solutions for Stellar Wind Torques","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":185,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Stellar wind; Torque; Stellar atmosphere; Computational astrophysics; Stellar structure; Stellar evolution; Stellar rotation","score_opus":0.01618369978741652,"score_gpt":0.23787907394793598,"score_spread":0.22169537416051946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975260087","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.11357737,0.01668839,0.69073635,0.0037732779,0.0028239691,0.00043595815,0.0011523475,0.000696019,0.17011629],"genre_scores_gemma":[0.7888512,0.0106340125,0.112366684,0.00049575855,0.0017975925,0.00069622864,0.0010117356,0.0006757785,0.08347103],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998692,0.000034657154,0.000011515838,0.000010100543,0.000056584857,0.000017768472],"domain_scores_gemma":[0.9996037,0.00014249593,0.000087077526,0.000037206686,0.00008986163,0.000039658815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055273436,0.00060618605,0.0006345768,0.00057775545,0.0004276836,0.001380283,0.00092479336,0.0015631156,0.0037570589],"category_scores_gemma":[0.0037913118,0.0005609358,0.000729381,0.000606684,0.0008873605,0.0007971807,0.0011307595,0.00097019644,0.0017063998],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055191864,0.00005337882,0.0014522979,0.00026601512,0.0000494258,0.000292915,0.00018790242,0.84146726,0.0025888095,0.11606268,0.0061748773,0.03134917],"study_design_scores_gemma":[0.00003235782,0.00001617122,0.0005847742,0.00006391312,0.000008056234,0.000073169416,0.000048232785,0.9650778,0.00037673407,0.027349714,0.0063556693,0.00001328806],"about_ca_topic_score_codex":0.0032266225,"about_ca_topic_score_gemma":0.0024414363,"teacher_disagreement_score":0.0037570589,"about_ca_system_score_codex":0.00058422267,"about_ca_system_score_gemma":0.00075250113,"threshold_uncertainty_score":0.012568593},"labels":[],"label_agreement":null},{"id":"W1975265017","doi":"10.1086/368122","title":"New Constraints on the Energetics, Progenitor Mass, and Age of the Supernova Remnant G292.0+1.8 Containing PSR J1124−5916","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Pulsar; Supernova remnant; Pulsar planet; Millisecond pulsar; RADIUS; Supernova; Crab Nebula; Neutron star; Ionization","score_opus":0.016430498786674453,"score_gpt":0.28309443979234855,"score_spread":0.2666639410056741,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975265017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967476,0.00057601946,0.0009854343,0.0000317941,0.000003906453,0.0000022590987,0.00015089844,0.00004003084,0.0014620977],"genre_scores_gemma":[0.99785537,0.00025041425,0.00084715144,0.000019399267,0.000012432887,0.0000028582144,0.00072355877,0.000012795368,0.00027596107],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999471,0.0000079200545,0.000005343805,0.000013266379,0.000014613351,0.00001172592],"domain_scores_gemma":[0.99964976,0.00009575288,0.00012399892,0.00005862698,0.000032777418,0.00003906941],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027497168,0.0003668801,0.00025043497,0.0005318553,0.00020993032,0.0005649032,0.00026688114,0.0003636634,0.0013202633],"category_scores_gemma":[0.00092641264,0.00020982328,0.00012882629,0.00035249002,0.00016731147,0.00043276616,0.00048482942,0.00023815311,0.0004153253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006705453,0.00015234057,0.4944054,0.00018923539,0.00011030879,0.002148782,0.0005978506,0.0050758766,0.46134907,0.0033105835,0.00080958137,0.031180445],"study_design_scores_gemma":[0.00006998282,0.00028199717,0.9315392,0.00003792568,0.00013474267,0.0036719367,0.0002519287,0.011246541,0.038785487,0.00439011,0.00955518,0.000035022174],"about_ca_topic_score_codex":0.0004551061,"about_ca_topic_score_gemma":0.0014152309,"teacher_disagreement_score":0.0013202633,"about_ca_system_score_codex":0.0001304261,"about_ca_system_score_gemma":0.00007646044,"threshold_uncertainty_score":0.004416764},"labels":[],"label_agreement":null},{"id":"W1975300467","doi":"10.1086/381162","title":"Point Sources in the Context of Future SZ Surveys","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Context (archaeology); South Pole Telescope; Radio telescope; Astronomy; Point source; James Clerk Maxwell Telescope; Galaxy cluster; Redshift; Telescope; Galaxy; Anisotropy; Star formation; Geography; Optics","score_opus":0.006639636848598921,"score_gpt":0.2059454179340248,"score_spread":0.19930578108542588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975300467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.85994714,0.014948021,0.060836744,0.02067977,0.00054592453,0.00012617085,0.0038231274,0.00045255793,0.03864059],"genre_scores_gemma":[0.9675245,0.009309762,0.014927067,0.00075602834,0.000759298,0.000047458565,0.0021115206,0.00004334719,0.0045210244],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99937755,0.00016150197,0.000025624531,0.00011038714,0.00022037093,0.000104536266],"domain_scores_gemma":[0.9952485,0.0016898959,0.00095604087,0.00041463083,0.0009985864,0.00069238164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016204054,0.00040120786,0.00045503385,0.0012371012,0.0005519557,0.0020836429,0.0007677049,0.000987685,0.0042372816],"category_scores_gemma":[0.007539006,0.0001745896,0.00029408472,0.0017908146,0.00056290085,0.0022904584,0.0016818582,0.001131932,0.0005988788],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047985735,0.00010103687,0.54017234,0.000712974,0.00018603136,0.0019376345,0.0017017289,0.0255911,0.0065289545,0.15353172,0.013505334,0.25555128],"study_design_scores_gemma":[0.00005394303,0.00038101137,0.7997829,0.00033095613,0.00016824089,0.0011103164,0.0033154658,0.026150793,0.003403108,0.10240863,0.06281425,0.00008043722],"about_ca_topic_score_codex":0.0055206246,"about_ca_topic_score_gemma":0.006006134,"teacher_disagreement_score":0.0055206246,"about_ca_system_score_codex":0.0008401638,"about_ca_system_score_gemma":0.0004448873,"threshold_uncertainty_score":0.014175177},"labels":[],"label_agreement":null},{"id":"W1975305731","doi":"10.1086/375484","title":"Global Parameter and Helioseismic Tests of Solar Variability Models","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Convection zone; Turbulence; Computational physics; Astrophysics; Turbulence kinetic energy; Radiation zone; Helioseismology; Magnetic energy; Radiative transfer; Convection; Magnetic field; Mechanics; Optics","score_opus":0.007978980400653705,"score_gpt":0.2267790182455849,"score_spread":0.2188000378449312,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975305731","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.990611,0.00012302687,0.0036673285,0.00021772592,0.000015266742,0.000013545798,0.0005574304,0.00012636776,0.004668296],"genre_scores_gemma":[0.9988545,0.00002795214,0.0004004981,0.000018676783,0.0000063167167,0.000009227884,0.0005720595,0.000021341562,0.000089438065],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99880886,0.00063261495,0.00006134907,0.00025567572,0.000113391165,0.00012818084],"domain_scores_gemma":[0.9903847,0.0064211846,0.0008339087,0.0013763568,0.0004890678,0.0004947983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0037928787,0.00081295316,0.0005098685,0.0005825726,0.00044529396,0.001316497,0.00093655183,0.0005539223,0.0029658054],"category_scores_gemma":[0.011807894,0.00021506546,0.0010467686,0.00066364766,0.0010734878,0.0015601045,0.0012842054,0.00053458737,0.00019633347],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014861315,0.00021081866,0.16727364,0.00009455714,0.0008405424,0.00022577112,0.00032976596,0.7971811,0.0014956977,0.01673784,0.001686772,0.012437372],"study_design_scores_gemma":[0.00058771914,0.0008205318,0.05310865,0.00003558593,0.00026175674,0.000119741344,0.00051596,0.91037375,0.0020468924,0.030067453,0.0020156754,0.00004625576],"about_ca_topic_score_codex":0.0036307857,"about_ca_topic_score_gemma":0.001953071,"teacher_disagreement_score":0.0037928787,"about_ca_system_score_codex":0.0009668635,"about_ca_system_score_gemma":0.0003715965,"threshold_uncertainty_score":0.02005893},"labels":[],"label_agreement":null},{"id":"W1975358219","doi":"10.1086/420898","title":"The Universality of Initial Conditions for Globular Cluster Formation","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Universality (dynamical systems); Homogeneous; Stellar density; Cluster (spacecraft); SPHERES; Star cluster; Isothermal process","score_opus":0.012958335319214961,"score_gpt":0.28363230589474075,"score_spread":0.2706739705755258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975358219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.903017,0.0004729169,0.07947072,0.00080803403,0.00008645827,0.00013480212,0.0004128479,0.0005565663,0.015040674],"genre_scores_gemma":[0.99564064,0.00015584992,0.0030691028,0.000053430806,0.000018988108,0.000039504557,0.00014118121,0.00007132684,0.00080993725],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9996927,0.000064047104,0.000012160445,0.000060693885,0.000056307832,0.0001142239],"domain_scores_gemma":[0.99895906,0.00032453984,0.00014685761,0.00017692342,0.0001402476,0.00025231333],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00075793907,0.0004253689,0.0006969496,0.000597544,0.0010030861,0.0011911211,0.0011898577,0.0013096237,0.002235834],"category_scores_gemma":[0.0078031607,0.0005014739,0.0010465557,0.00036364744,0.0015358903,0.0017798701,0.0012661073,0.0008846552,0.000358013],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013722382,0.0000934085,0.027342306,0.000098396034,0.000085808955,0.0008800737,0.0007826008,0.8001938,0.008458446,0.15544385,0.0013251036,0.0051589576],"study_design_scores_gemma":[0.00011623336,0.00011683015,0.010858842,0.000029673885,0.000038950344,0.00027713718,0.00021227011,0.8949628,0.0020412891,0.089860536,0.0014217984,0.000063553685],"about_ca_topic_score_codex":0.01442484,"about_ca_topic_score_gemma":0.00534766,"teacher_disagreement_score":0.01442484,"about_ca_system_score_codex":0.001944147,"about_ca_system_score_gemma":0.0014211627,"threshold_uncertainty_score":0.028681755},"labels":[],"label_agreement":null},{"id":"W1975379205","doi":"10.1086/524398","title":"The Red‐Sequence Luminosity Function in Galaxy Clusters since<i>z</i>∼ 1","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Waterloo","funders":"","keywords":"Astrophysics; Physics; Astronomy; Galaxy cluster; Redshift; Elliptical galaxy; Luminosity function; Brightest cluster galaxy; Galaxy; Lenticular galaxy; Galaxy formation and evolution; Star formation","score_opus":0.012435894421395711,"score_gpt":0.20931841549749683,"score_spread":0.19688252107610113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975379205","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945326,0.0002590594,0.00013229995,0.00014889885,0.000007649391,0.000003039124,0.001484632,0.000040154468,0.0033916607],"genre_scores_gemma":[0.9967458,0.000055734443,0.00005673742,0.000028823544,0.000006437164,0.0000029474916,0.001640937,0.000008727159,0.0014538132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998659,0.000013112081,0.0000049464024,0.000044355955,0.000016658327,0.000055002656],"domain_scores_gemma":[0.9977664,0.00031719074,0.0005535414,0.00012393124,0.00034648046,0.0008924888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033279235,0.00012277394,0.00015236667,0.0016972471,0.0004412872,0.0009025963,0.00039683652,0.00050370104,0.005444811],"category_scores_gemma":[0.0024230047,0.00012920742,0.00020275405,0.001028373,0.0003510751,0.00044645683,0.0005755479,0.0003638852,0.0014017039],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013106261,0.00002646625,0.9888242,0.000011547758,0.000022638324,0.000038974245,0.00033703077,0.0006389441,0.0009564284,0.0006654043,0.0019447643,0.006402537],"study_design_scores_gemma":[8.3198694e-7,0.0000067339197,0.99929905,0.000002093874,0.0000024492408,0.000019613923,0.00007409838,0.00020153556,0.000029441795,0.00006764303,0.00029470772,0.0000016836099],"about_ca_topic_score_codex":0.08131499,"about_ca_topic_score_gemma":0.07746859,"teacher_disagreement_score":0.08131499,"about_ca_system_score_codex":0.00088783284,"about_ca_system_score_gemma":0.0004359066,"threshold_uncertainty_score":0.16168332},"labels":[],"label_agreement":null},{"id":"W1975513891","doi":"10.1086/429790","title":"High‐Mass Star Formation. I. The Mass Distribution of Submillimeter Clumps in NGC 7538","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"James Clerk Maxwell Telescope; Physics; Astrophysics; Bolometer; Millimeter; Star formation; Spectral index; Mass distribution; Submillimeter Array; Astronomy; Power law; Telescope; Galaxy; Far infrared; Molecular cloud; RADIUS; Infrared; Stars; Spectral line; Optics","score_opus":0.008404233704972024,"score_gpt":0.22086793898404394,"score_spread":0.2124637052790719,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975513891","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99910694,0.00006927543,0.000062713,0.000009635564,7.142398e-7,0.0000020293544,0.00012818424,0.000011471798,0.0006090143],"genre_scores_gemma":[0.99967504,0.00001695797,0.000103335435,0.000003580178,0.0000017192319,0.0000017346538,0.00010661322,0.0000017309835,0.000089395005],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999168,0.00000406787,0.000004884415,0.000025352423,0.000018465136,0.000030476544],"domain_scores_gemma":[0.9997069,0.000026544974,0.00013195186,0.00002638209,0.000028476916,0.000079696125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008880045,0.000195371,0.0001839785,0.00082814856,0.0003051615,0.00038414684,0.00027731538,0.00015842338,0.0011535436],"category_scores_gemma":[0.00032672286,0.00012598552,0.00013409881,0.0005129749,0.00029321847,0.00019474443,0.00043557948,0.00016299871,0.00029211075],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000819742,0.0000231394,0.96386063,0.000023711145,0.000024341964,0.0003286689,0.0005844763,0.0005848839,0.025666675,0.00021564253,0.0002862158,0.008319558],"study_design_scores_gemma":[0.000002011195,0.000010415714,0.99902284,0.0000022998072,0.0000028103996,0.00010229694,0.0000675363,0.00020616873,0.00031858243,0.00003221606,0.00023092312,0.0000018108378],"about_ca_topic_score_codex":0.013808385,"about_ca_topic_score_gemma":0.014914831,"teacher_disagreement_score":0.013808385,"about_ca_system_score_codex":0.00051740167,"about_ca_system_score_gemma":0.0000862282,"threshold_uncertainty_score":0.027455986},"labels":[],"label_agreement":null},{"id":"W1975554241","doi":"10.1088/0004-637x/772/2/82","title":"A CATALOG OF GLOBULAR CLUSTER SYSTEMS: WHAT DETERMINES THE SIZE OF A GALAXY'S GLOBULAR CLUSTER POPULATION?","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":309,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; McMaster University","funders":"","keywords":"Globular cluster; Velocity dispersion; Galaxy cluster; Galaxy; Luminosity; Brightest cluster galaxy; Interacting galaxy; Type-cD galaxy; Galaxy groups and clusters","score_opus":0.005575716491502924,"score_gpt":0.20644902338622265,"score_spread":0.20087330689471972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975554241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9167196,0.0024625894,0.0037852263,0.0005663875,0.0000448,0.00008893542,0.059649944,0.0007315569,0.015950939],"genre_scores_gemma":[0.9248142,0.002069489,0.008315349,0.00017246554,0.00013250028,0.00009223742,0.061212905,0.00006834145,0.003122513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972874,0.000037274458,0.00003394308,0.00007307811,0.00009952575,0.000027408943],"domain_scores_gemma":[0.99682164,0.00062267185,0.00074000336,0.00043421524,0.00093618204,0.0004454075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006122438,0.00024165129,0.00027666942,0.006864841,0.00033958285,0.0010635508,0.00041604033,0.00033925928,0.0045136563],"category_scores_gemma":[0.0029998217,0.00014825209,0.00013966164,0.007506047,0.00026612217,0.0010856402,0.00037549893,0.00016894197,0.0020817777],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042350206,0.000030100555,0.9463947,0.00013071907,0.000051296367,0.000072043775,0.00015824295,0.000546135,0.0013583595,0.00088077114,0.008372976,0.04196233],"study_design_scores_gemma":[0.0000068411587,0.000034528955,0.98834395,0.000028086357,0.000027043969,0.00025100823,0.00017819002,0.0010362146,0.0003428256,0.00037610286,0.0093649775,0.000010286125],"about_ca_topic_score_codex":0.008735394,"about_ca_topic_score_gemma":0.01328109,"teacher_disagreement_score":0.008735394,"about_ca_system_score_codex":0.00032249675,"about_ca_system_score_gemma":0.000492571,"threshold_uncertainty_score":0.017369092},"labels":[],"label_agreement":null},{"id":"W1975617105","doi":"10.1088/0004-637x/716/1/792","title":"DEEP<i>K<sub>s</sub></i>-NEAR-INFRARED SURFACE PHOTOMETRY OF 80 DWARF IRREGULAR GALAXIES IN THE LOCAL VOLUME","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Astronomy; Infrared astronomy; Infrared; Galaxy; Dwarf galaxy; Luminous infrared galaxy; Stars","score_opus":0.004627321068143565,"score_gpt":0.1984046088331373,"score_spread":0.19377728776499373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975617105","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99867463,0.000037168844,0.00019263286,0.000006319122,6.984908e-7,0.0000020526654,0.0003870725,0.000028499891,0.00067091547],"genre_scores_gemma":[0.99722314,0.000037452683,0.0009321056,0.0000098345245,0.0000025583352,0.0000027418569,0.0012982365,0.0000106038015,0.00048323208],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994314,0.000003145591,0.0000039306356,0.000018100023,0.000012690209,0.000018985764],"domain_scores_gemma":[0.99965096,0.000027239525,0.0001332257,0.00004446427,0.000040794424,0.00010330704],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010342313,0.000151334,0.00014432645,0.00070717814,0.00018808772,0.00020831783,0.00016990642,0.0001237581,0.0009327938],"category_scores_gemma":[0.00023595465,0.00013501209,0.000102247475,0.00048070925,0.00020700805,0.00021836841,0.0003667049,0.00012881536,0.00031800804],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027449225,0.000053940224,0.91749656,0.000033226283,0.000046637233,0.00017005003,0.00041546108,0.0008673209,0.056662094,0.00012846853,0.0006588524,0.023192745],"study_design_scores_gemma":[0.000002671517,0.000024393727,0.99700314,0.0000012782824,0.0000070163537,0.00010649642,0.000069550064,0.00034877632,0.0018673565,0.000028219389,0.0005382607,0.0000028249692],"about_ca_topic_score_codex":0.0033752795,"about_ca_topic_score_gemma":0.0120971985,"teacher_disagreement_score":0.0033752795,"about_ca_system_score_codex":0.00024920283,"about_ca_system_score_gemma":0.00007611997,"threshold_uncertainty_score":0.006711304},"labels":[],"label_agreement":null},{"id":"W1975666791","doi":"10.1086/423418","title":"A High Spatial Resolution Infrared View of the T Tauri Multiple System","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; T Tauri star; Brightness; Extinction (optical mineralogy); Line (geometry); Infrared; Line-of-sight; Light curve; Astronomy; Optics; Geometry; Stars","score_opus":0.008252668314220255,"score_gpt":0.20980097145481047,"score_spread":0.20154830314059022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975666791","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9220959,0.0016408649,0.010974815,0.00033840403,0.00006174473,0.00003947327,0.0017397641,0.00066740037,0.062441498],"genre_scores_gemma":[0.9847772,0.0005757456,0.0097069,0.00010605899,0.00020488296,0.000015855027,0.0008018716,0.00006731163,0.003744239],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999474,0.0000037995487,0.0000020079083,0.00001279842,0.00001969366,0.000014294018],"domain_scores_gemma":[0.9998733,0.000015457968,0.000030051653,0.0000148763065,0.000020500347,0.000045850316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000091246984,0.00015680074,0.00009638913,0.0012841431,0.00032528976,0.00039963308,0.00022414884,0.0001969402,0.0044435486],"category_scores_gemma":[0.00013259423,0.00013442193,0.00015969145,0.00055966986,0.00009906437,0.000380607,0.00033356453,0.0004816926,0.00086757704],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071009074,0.0003809775,0.123773314,0.00029761725,0.00011735464,0.0047822916,0.0013680069,0.004609795,0.6705908,0.0033662098,0.0100289,0.17997468],"study_design_scores_gemma":[0.000029008712,0.00033359876,0.953989,0.000058189395,0.000060872953,0.007294229,0.0003815382,0.0066776597,0.0097329,0.001012788,0.020404618,0.00002539286],"about_ca_topic_score_codex":0.0012095437,"about_ca_topic_score_gemma":0.00204882,"teacher_disagreement_score":0.0044435486,"about_ca_system_score_codex":0.00011884871,"about_ca_system_score_gemma":0.00009031793,"threshold_uncertainty_score":0.01486516},"labels":[],"label_agreement":null},{"id":"W1975717686","doi":"10.1088/0004-637x/768/2/115","title":"GENERAL-RELATIVISTIC SIMULATIONS OF THREE-DIMENSIONAL CORE-COLLAPSE SUPERNOVAE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":191,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; California Institute of Technology; Alfred P. Sloan Foundation; Sherman Fairchild Foundation; National Science Foundation","keywords":"Physics; Neutrino; Instability; Supernova; Convection; Type II supernova; Mechanics; Astrophysics; Nuclear physics","score_opus":0.015068233553182268,"score_gpt":0.2308580597691984,"score_spread":0.21578982621601614,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975717686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9827466,0.00018541976,0.0069517395,0.00041665332,0.00006133505,0.00005977975,0.00083954807,0.0003021975,0.008436663],"genre_scores_gemma":[0.99149686,0.00013838963,0.006087649,0.00014712883,0.00002882037,0.000074745796,0.00089310174,0.00008319973,0.0010500348],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99978,0.000057495916,0.000012091817,0.000028883149,0.00004995813,0.000071620096],"domain_scores_gemma":[0.99887615,0.00047688576,0.0001661121,0.00007329353,0.00017101201,0.0002365617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005025276,0.0006955267,0.0007780945,0.00055821094,0.0006888808,0.0007432151,0.0017353278,0.0012257128,0.0021692023],"category_scores_gemma":[0.0022655786,0.00047301446,0.0010851951,0.000818284,0.0010336102,0.00037026303,0.001138552,0.0011453185,0.0001804155],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012835718,0.000104156185,0.0040923934,0.00003146758,0.000054785418,0.00010890582,0.00007020372,0.99151576,0.0009106779,0.0017625666,0.0002679958,0.000952645],"study_design_scores_gemma":[0.000048114205,0.000035551802,0.0015395804,0.0000040674545,0.000009904442,0.000010776135,0.000030770192,0.997391,0.0002024635,0.0005306562,0.00018807944,0.000009025686],"about_ca_topic_score_codex":0.037424497,"about_ca_topic_score_gemma":0.016917935,"teacher_disagreement_score":0.037424497,"about_ca_system_score_codex":0.0013441113,"about_ca_system_score_gemma":0.0010488109,"threshold_uncertainty_score":0.07441336},"labels":[],"label_agreement":null},{"id":"W1975745420","doi":"10.1086/323357","title":"<i>Hubble Space Telescope</i>Imagery and Canada‐France‐Hawaii Telescope Fabry‐Perot Two‐dimensional Spectroscopy in Hα of the Ejected Nebula M1‐67: Turbulent Status","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université Laval; Canada Council for the Arts; Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Nebula; Astronomy; Stars; Planetary nebula; Proper motion; Galaxy; Emission nebula; Context (archaeology)","score_opus":0.005370835873083611,"score_gpt":0.20715303329403245,"score_spread":0.20178219742094883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975745420","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3500594,0.0018189261,0.005930258,0.002833343,0.0005580157,0.00036098983,0.36081198,0.005618048,0.27200907],"genre_scores_gemma":[0.6964409,0.001928879,0.029073838,0.0008444476,0.00031525883,0.00016894475,0.21026562,0.00093569845,0.06002648],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99990964,0.000005841518,0.0000041308126,0.000013413503,0.000039199575,0.000027735596],"domain_scores_gemma":[0.9996321,0.000017264605,0.00007799766,0.000051658626,0.00014061086,0.00008022469],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012790265,0.0003019572,0.00015557537,0.0025210453,0.00043511594,0.00067873485,0.0004053633,0.00027409798,0.027206702],"category_scores_gemma":[0.00039128942,0.00011413511,0.00012637163,0.0021426578,0.0002503366,0.00028111783,0.00032944183,0.00037230196,0.0055189906],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004473837,0.00009929078,0.14779897,0.0005778171,0.0000996811,0.00092913845,0.0010073273,0.0012080161,0.08806233,0.0037361472,0.5942482,0.1617857],"study_design_scores_gemma":[0.0000183826,0.000017521706,0.8114143,0.00007016086,0.000013309576,0.00030193556,0.00030521877,0.0008643519,0.0037622221,0.00019472184,0.18301874,0.000019276433],"about_ca_topic_score_codex":0.22325559,"about_ca_topic_score_gemma":0.3753532,"teacher_disagreement_score":0.22325559,"about_ca_system_score_codex":0.0010570684,"about_ca_system_score_gemma":0.00071217655,"threshold_uncertainty_score":0.44391215},"labels":[],"label_agreement":null},{"id":"W1975769275","doi":"10.1088/0004-637x/787/2/104","title":"A FIRST-LOOK ATMOSPHERIC MODELING STUDY OF THE YOUNG DIRECTLY IMAGED PLANET-MASS COMPANION, ROXS 42Bb","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Photometry (optics); Physics; Planetary mass; Astrophysics; Planet; Brown dwarf; Astronomy; Surface gravity; Spectral slope; Spectral index; Effective temperature; Spectral line; Planetary system; Stars","score_opus":0.00846788064251653,"score_gpt":0.213074106749036,"score_spread":0.2046062261065195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975769275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897187,0.00020706303,0.0029287888,0.0003308801,0.000024772879,0.00001988735,0.0013183914,0.00035890943,0.005092652],"genre_scores_gemma":[0.99443454,0.00011530646,0.003201107,0.000046607624,0.000022681037,0.000009210289,0.0012173362,0.000075477816,0.0008778125],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999931,0.000008768617,0.0000020654415,0.000032294556,0.000011861167,0.000014014428],"domain_scores_gemma":[0.9998821,0.000018147417,0.000017680162,0.000017932982,0.000025045034,0.000039101604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020258401,0.00041335667,0.0002801653,0.0003991402,0.00074254855,0.0006203064,0.00086713413,0.0005343752,0.0012762017],"category_scores_gemma":[0.00031328952,0.00020691927,0.00047172734,0.00034419398,0.00016125616,0.00067864504,0.00037277467,0.00048506242,0.00039955464],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047209644,0.0009292403,0.61093974,0.00015259915,0.00038137,0.001448283,0.0014086457,0.2964168,0.026724463,0.008368644,0.0122696785,0.040488504],"study_design_scores_gemma":[0.00008512699,0.00016530982,0.13708557,0.000013274577,0.00010976484,0.00046289124,0.0006490016,0.84477115,0.0028058577,0.0013032518,0.012499673,0.000049139057],"about_ca_topic_score_codex":0.0630609,"about_ca_topic_score_gemma":0.05364067,"teacher_disagreement_score":0.0630609,"about_ca_system_score_codex":0.0007095287,"about_ca_system_score_gemma":0.00047303858,"threshold_uncertainty_score":0.12538773},"labels":[],"label_agreement":null},{"id":"W1975777470","doi":"10.1088/0004-637x/768/2/172","title":"A KINEMATIC STUDY OF THE ANDROMEDA DWARF SPHEROIDAL SYSTEM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":182,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Dalhousie University","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Milky Way; Local Group; Dwarf spheroidal galaxy; Velocity dispersion; Andromeda; Red-giant branch; Dark matter; Astronomy; Population; Globular cluster; Andromeda Galaxy; Galaxy; Radial velocity; Dark matter halo; Metallicity; Stars; Dwarf galaxy; Halo","score_opus":0.009332427308113407,"score_gpt":0.2094037988936428,"score_spread":0.2000713715855294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975777470","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955389,0.00043183813,0.00076653395,0.000014743989,0.0000020019518,0.000008593689,0.00044272142,0.000021972333,0.0027726132],"genre_scores_gemma":[0.99590683,0.00026696207,0.002036258,0.0000054559705,0.000010231915,0.0000046683767,0.0010874993,0.000007952318,0.0006740943],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986076,0.00002871782,0.000009259089,0.0000519731,0.000023958648,0.000025232934],"domain_scores_gemma":[0.99974555,0.000027784916,0.00009411509,0.00003106586,0.000041877098,0.000059589387],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015834786,0.00024053207,0.00018432949,0.001421016,0.00035219494,0.00044997895,0.00020662766,0.00006574635,0.0011514192],"category_scores_gemma":[0.0004317626,0.00008765683,0.00017970061,0.0011269845,0.0002031492,0.00021060336,0.00031249394,0.00010494,0.00046787827],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009585845,0.000034648234,0.9621933,0.000021880584,0.000040762185,0.0003015062,0.0006554247,0.000872921,0.009473607,0.0009393685,0.0002551768,0.025115568],"study_design_scores_gemma":[0.0000031988222,0.000054556203,0.99367946,0.000006240025,0.000013278959,0.00072321395,0.00025202797,0.001224104,0.0007237048,0.00017204478,0.00314148,0.0000067013284],"about_ca_topic_score_codex":0.010417276,"about_ca_topic_score_gemma":0.013221075,"teacher_disagreement_score":0.010417276,"about_ca_system_score_codex":0.0003026587,"about_ca_system_score_gemma":0.00024684117,"threshold_uncertainty_score":0.02071327},"labels":[],"label_agreement":null},{"id":"W1975777954","doi":"10.1088/0004-637x/726/1/48","title":"THE MASS-<i>L<sub>x</sub></i>RELATION FOR MODERATE LUMINOSITY X-RAY CLUSTERS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"ROSAT; Galaxy; Cluster (spacecraft); Weak gravitational lensing; Luminosity; Galaxy cluster; Scaling; Power law; Galaxy groups and clusters","score_opus":0.006196470226465156,"score_gpt":0.20168878585410546,"score_spread":0.1954923156276403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975777954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977323,0.0002201752,0.0006910238,0.000032931155,0.0000016470117,0.0000028187894,0.00035958074,0.000043155207,0.00091625005],"genre_scores_gemma":[0.99892336,0.000044485838,0.0005299567,0.000007883537,0.000005024973,0.0000043295836,0.00037671183,0.000007029498,0.00010116123],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980897,0.000022761726,0.000017392107,0.00008501029,0.000034971697,0.00003097127],"domain_scores_gemma":[0.9979086,0.0004192066,0.0011168517,0.00020997012,0.0001386401,0.0002068738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027863492,0.000271958,0.00018813813,0.0012801382,0.00027987323,0.000525532,0.00033451864,0.0002668063,0.0011059954],"category_scores_gemma":[0.0021903818,0.0002282593,0.00014301405,0.0006846991,0.00034084063,0.00043121818,0.00059347367,0.00027771306,0.0004567674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001248152,0.000013212458,0.98201895,0.00003052393,0.000040676903,0.000054510052,0.00020121642,0.0009083181,0.010453465,0.00072442886,0.00032744918,0.00510245],"study_design_scores_gemma":[0.0000049009764,0.000044131513,0.99503434,0.000005122175,0.0000140827915,0.00023246261,0.000059798716,0.0014426295,0.0021383052,0.0004414149,0.0005735837,0.000009210916],"about_ca_topic_score_codex":0.0013335992,"about_ca_topic_score_gemma":0.0017661613,"teacher_disagreement_score":0.0013335992,"about_ca_system_score_codex":0.00030962948,"about_ca_system_score_gemma":0.00008198521,"threshold_uncertainty_score":0.0036998987},"labels":[],"label_agreement":null},{"id":"W1975827586","doi":"10.1086/421464","title":"Formation and Collapse of Nonaxisymmetric Protostellar Cores in Planar Magnetic Molecular Clouds","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Physics; Gravitational collapse; Supercritical fluid; Molecular cloud; Supersonic speed; Astrophysics; Mechanics; Plasma; Nuclear physics; Thermodynamics","score_opus":0.006698218720272817,"score_gpt":0.21927039120132433,"score_spread":0.2125721724810515,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1975827586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992299,0.00002542037,0.00028470074,0.000010135022,8.7445835e-7,0.0000033635833,0.00001279674,0.0000064417336,0.0004263754],"genre_scores_gemma":[0.99969745,0.000021189007,0.00016646383,0.0000036035,9.263781e-7,0.0000018346975,0.00002959451,0.0000018338578,0.00007714041],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995816,0.0000042504025,0.0000017120279,0.000007949663,0.000010128645,0.000017790742],"domain_scores_gemma":[0.9998367,0.000017473922,0.000064839645,0.00001325275,0.00001065187,0.000057106583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000064872336,0.00017687463,0.00014824925,0.0002509211,0.00037927608,0.0004516203,0.0003261356,0.0002163841,0.0003492596],"category_scores_gemma":[0.00038609948,0.00016164134,0.00018347256,0.00012830882,0.00036507018,0.0002861458,0.0005385258,0.00019088105,0.000054240467],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007336003,0.0003840868,0.18765125,0.00012050483,0.00016470728,0.0024209064,0.0008163183,0.3108976,0.46742034,0.017820297,0.0006306657,0.010939722],"study_design_scores_gemma":[0.00023664701,0.00064826006,0.20873733,0.00001269277,0.000047874204,0.0008491272,0.0005146515,0.69577026,0.08581392,0.005818724,0.0015118378,0.000038681443],"about_ca_topic_score_codex":0.0053647994,"about_ca_topic_score_gemma":0.004817007,"teacher_disagreement_score":0.0053647994,"about_ca_system_score_codex":0.00070930255,"about_ca_system_score_gemma":0.00030159872,"threshold_uncertainty_score":0.010667145},"labels":[],"label_agreement":null},{"id":"W1976036221","doi":"10.1086/341435","title":"Is There Evidence for Rotation or Horizontal Motions in Hot DB White Dwarfs?","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; White dwarf; Spectrograph; Astrophysics; Rotation (mathematics); Astronomy; Radial velocity; Stars; Spectral line; Geometry","score_opus":0.05125347941028944,"score_gpt":0.2810259908994184,"score_spread":0.22977251148912894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976036221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996573,0.0014642797,0.00027761862,0.00030158908,0.000014483789,0.0000021217195,0.000052821033,0.000014445839,0.0012997307],"genre_scores_gemma":[0.9989083,0.0005894741,0.00009961787,0.00010769268,0.00004104706,0.0000015431854,0.00007678435,0.0000024470507,0.00017319254],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997986,0.00002561712,0.000016812777,0.00004316967,0.0000377629,0.0000779986],"domain_scores_gemma":[0.9988757,0.00022113099,0.00051247753,0.00008513432,0.00009952203,0.0002059835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037901293,0.00020654041,0.000347695,0.00066547963,0.00043225117,0.0006312861,0.00028059888,0.00051347027,0.0015479325],"category_scores_gemma":[0.001390121,0.00014716336,0.00019245454,0.00061527506,0.0013850848,0.00061030407,0.00039364406,0.00018354185,0.00043105177],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022089109,0.000027267082,0.9637024,0.00008793608,0.00004786202,0.00088711304,0.00037855026,0.000049120175,0.018657686,0.00040743928,0.00014383106,0.015389978],"study_design_scores_gemma":[0.000009927692,0.00010114673,0.99383754,0.000015674064,0.000029203358,0.0017012309,0.0006207054,0.000070605274,0.0020968567,0.00046515718,0.0010466481,0.000005365291],"about_ca_topic_score_codex":0.002352559,"about_ca_topic_score_gemma":0.0025723174,"teacher_disagreement_score":0.002352559,"about_ca_system_score_codex":0.00023232393,"about_ca_system_score_gemma":0.00020054358,"threshold_uncertainty_score":0.0051783323},"labels":[],"label_agreement":null},{"id":"W1976071602","doi":"10.1088/0004-637x/719/2/1896","title":"THE BURST MODE OF ACCRETION AND DISK FRAGMENTATION IN THE EARLY EMBEDDED STAGES OF STAR FORMATION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":319,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Protostar; Radiative transfer; Accretion (finance); Angular momentum; Star formation; Circumstellar disk; Fragmentation (computing); Astronomy; Planet; Stars; Classical mechanics","score_opus":0.007502614009947908,"score_gpt":0.25623288934709687,"score_spread":0.24873027533714898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976071602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6058898,0.010540886,0.34492826,0.0012718282,0.00028531917,0.00012445904,0.00033090977,0.00022803863,0.036400504],"genre_scores_gemma":[0.9669921,0.00283696,0.018822713,0.00016799304,0.0002578323,0.00006192567,0.000082031154,0.000052536645,0.010725804],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998568,0.000025838901,0.000011876801,0.00003955126,0.00003313035,0.000032720734],"domain_scores_gemma":[0.99962866,0.000085386724,0.00013258582,0.000056745015,0.000042222837,0.000054347096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003723114,0.00045292763,0.00033573655,0.00044026744,0.00027242693,0.00080766715,0.0013138502,0.0007384004,0.0016167093],"category_scores_gemma":[0.00072714104,0.00019784739,0.0006223785,0.00027615528,0.000578515,0.0012513871,0.0007664004,0.0005963529,0.00035669084],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033009608,0.0001760185,0.07948758,0.00078834424,0.00019681203,0.0040155873,0.0032058866,0.15064244,0.05011186,0.6049253,0.0033579466,0.10276215],"study_design_scores_gemma":[0.000085930915,0.00048832654,0.059565257,0.00025534243,0.00010561763,0.0048208307,0.0007086651,0.6092335,0.008537176,0.26616883,0.049931593,0.00009883055],"about_ca_topic_score_codex":0.0017996236,"about_ca_topic_score_gemma":0.0009231344,"teacher_disagreement_score":0.0017996236,"about_ca_system_score_codex":0.0005543652,"about_ca_system_score_gemma":0.00035487826,"threshold_uncertainty_score":0.005408466},"labels":[],"label_agreement":null},{"id":"W1976122525","doi":"10.1086/512802","title":"Measuring PAH Emission in Ultradeep<i>Spitzer</i>IRS Spectroscopy of High‐Redshift IR‐Luminous Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Spitzer Space Telescope; Galaxy; Redshift; Astronomy; Luminosity; Star formation; Luminous infrared galaxy; Emission spectrum; Population; Spectrograph; Stars; Spectral line","score_opus":0.009383548030126808,"score_gpt":0.21324944278021937,"score_spread":0.20386589475009256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976122525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99761933,0.000104839135,0.0005257838,0.000016816497,0.00000308381,0.000003861466,0.00014851615,0.00003437895,0.001543307],"genre_scores_gemma":[0.99830097,0.0001077153,0.0007043003,0.00003807295,0.000010108793,0.000005921291,0.00032697953,0.000007994944,0.0004979641],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991417,0.0000070749265,0.0000029869427,0.000030379368,0.000020756166,0.000024648014],"domain_scores_gemma":[0.99978215,0.00003874729,0.00007725052,0.000020202728,0.0000339791,0.00004767871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018130052,0.00020078695,0.00014879733,0.0008518464,0.00026109794,0.00045440558,0.00035872377,0.00027672906,0.0009435586],"category_scores_gemma":[0.0002619442,0.00021194557,0.00014649356,0.00043586027,0.0001925823,0.00041712486,0.00029806473,0.00028906163,0.00027151266],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037079633,0.0001988683,0.3455342,0.000048387483,0.00008737601,0.00023325447,0.0002769058,0.00054773706,0.6397537,0.00045502893,0.0003440743,0.012149619],"study_design_scores_gemma":[0.000007249363,0.000062293286,0.9829858,0.0000039536117,0.000024768018,0.00016004869,0.000072924275,0.00048548167,0.0158112,0.00005861726,0.000322665,0.0000050187296],"about_ca_topic_score_codex":0.001016673,"about_ca_topic_score_gemma":0.0024039918,"teacher_disagreement_score":0.001016673,"about_ca_system_score_codex":0.00015550507,"about_ca_system_score_gemma":0.000076809316,"threshold_uncertainty_score":0.0031565428},"labels":[],"label_agreement":null},{"id":"W1976166792","doi":"10.1086/591899","title":"<i>Chandra X‐Ray Observatory</i>Observations of the Globular Cluster M71","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Alberta","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Millisecond pulsar; Observatory; RADIUS; Luminosity; Astronomy; Pulsar; Light curve; Cluster (spacecraft); Neutron star; Galaxy","score_opus":0.02341841813007581,"score_gpt":0.2199268006943075,"score_spread":0.1965083825642317,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976166792","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.18206331,0.0123670865,0.0049081845,0.011771793,0.018393505,0.00054221525,0.4927278,0.0072520594,0.26997402],"genre_scores_gemma":[0.33704537,0.0064392486,0.0051713954,0.002229387,0.0050945133,0.00012993078,0.51172197,0.0010307243,0.13113749],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99965525,0.000010948213,0.000025422072,0.00005568483,0.00014467147,0.000108088585],"domain_scores_gemma":[0.99849236,0.000111150235,0.00028596545,0.00044064614,0.00045545524,0.00021446233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005142669,0.00046704302,0.00055511046,0.0042466912,0.0012461946,0.0020798866,0.00084680045,0.00095261505,0.061190296],"category_scores_gemma":[0.0019354417,0.00041109495,0.00055706315,0.004005038,0.00040253322,0.0014943186,0.0014688631,0.0010983151,0.018665588],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00223242,0.00022557202,0.025055423,0.0023870892,0.00029880146,0.0008921253,0.00025567607,0.0009917647,0.030413857,0.008208692,0.8261638,0.10287475],"study_design_scores_gemma":[0.00015668449,0.00012035893,0.36314756,0.0003072887,0.0001596755,0.0004677737,0.00009342132,0.00030745516,0.005426638,0.0010936452,0.6286228,0.0000967674],"about_ca_topic_score_codex":0.019049006,"about_ca_topic_score_gemma":0.03909682,"teacher_disagreement_score":0.061190296,"about_ca_system_score_codex":0.0013981028,"about_ca_system_score_gemma":0.0016344447,"threshold_uncertainty_score":0.2047019},"labels":[],"label_agreement":null},{"id":"W1976229996","doi":"10.1088/0004-637x/783/2/107","title":"RADIAL STELLAR PULSATION AND THREE-DIMENSIONAL CONVECTION. III. COMPARISON OF TWO-DIMENSIONAL AND THREE-DIMENSIONAL CONVECTION EFFECTS ON RADIAL PULSATION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Convection; Physics; Amplitude; Stellar pulsation; Light curve; RR Lyrae variable; Mechanics; Astrophysics; Stars; Computational physics; Optics","score_opus":0.01042604288276455,"score_gpt":0.23590145628452794,"score_spread":0.22547541340176339,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976229996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97254723,0.00027343837,0.019728752,0.0002901773,0.0000685497,0.00005006157,0.00034134617,0.000578742,0.0061216694],"genre_scores_gemma":[0.99409807,0.00008871505,0.0049379272,0.00005915775,0.000014793458,0.000033506054,0.00014640288,0.000103779545,0.00051765563],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981636,0.00005696922,0.000019236952,0.000021074713,0.00005018998,0.0000362962],"domain_scores_gemma":[0.99886143,0.00056362164,0.00017544108,0.00012092239,0.00016212593,0.00011650551],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046829256,0.0006000767,0.0004641376,0.00038142552,0.00040343017,0.0008396744,0.00067699864,0.0006988488,0.0011608314],"category_scores_gemma":[0.0025488846,0.0004018854,0.00096796395,0.00037032462,0.00059999776,0.00073604967,0.0008847256,0.000718637,0.00018714496],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012555838,0.00009463735,0.0092140455,0.000071022674,0.000065112,0.00016356967,0.00009518378,0.9701745,0.015018274,0.0018931297,0.00017538593,0.0029095488],"study_design_scores_gemma":[0.000036389367,0.000031104435,0.0018716187,0.000005049502,0.000008370336,0.00002281351,0.000011656835,0.99443984,0.0031774412,0.00021999996,0.00016152266,0.000014200356],"about_ca_topic_score_codex":0.007135901,"about_ca_topic_score_gemma":0.0020771914,"teacher_disagreement_score":0.007135901,"about_ca_system_score_codex":0.00071714213,"about_ca_system_score_gemma":0.0006533699,"threshold_uncertainty_score":0.014188707},"labels":[],"label_agreement":null},{"id":"W1976269218","doi":"10.1088/0004-637x/728/2/116","title":"THE ACS FORNAX CLUSTER SURVEY. X. COLOR GRADIENTS OF GLOBULAR CLUSTER SYSTEMS IN EARLY-TYPE GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Galaxy; Fornax Cluster; Cluster (spacecraft); Stars; Star cluster; Galaxy cluster; Star formation","score_opus":0.015922387739099327,"score_gpt":0.21641690741977315,"score_spread":0.20049451968067383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976269218","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.061115734,0.0017900863,0.00021676027,0.0017361033,0.00020238392,0.00012410134,0.90692985,0.0007919466,0.027093058],"genre_scores_gemma":[0.17977127,0.001674928,0.0024317915,0.00067876425,0.0002536331,0.0003428784,0.77582926,0.0002612462,0.03875621],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9997613,0.000024547864,0.000021558428,0.000059856142,0.00007689252,0.000055812285],"domain_scores_gemma":[0.9987544,0.000085547166,0.00032540984,0.00012072509,0.00037558927,0.0003383701],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005407863,0.00036492266,0.00032971642,0.005488267,0.0007177089,0.0007195042,0.0007347769,0.00044938998,0.027940163],"category_scores_gemma":[0.0015438006,0.00022922066,0.000244871,0.004750231,0.00020126266,0.0009502288,0.0011119472,0.00047971567,0.009365977],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001840939,0.00008191694,0.16407062,0.00024528784,0.000085189815,0.000052124076,0.0002259249,0.00013003382,0.00054739724,0.0010861707,0.8009731,0.03231821],"study_design_scores_gemma":[0.00007242592,0.00002018343,0.8825032,0.00006393175,0.000029117793,0.000048744812,0.00032155964,0.000093339164,0.00012913696,0.00027328308,0.11643246,0.000012497232],"about_ca_topic_score_codex":0.16121326,"about_ca_topic_score_gemma":0.2013529,"teacher_disagreement_score":0.16121326,"about_ca_system_score_codex":0.0009593497,"about_ca_system_score_gemma":0.00095287734,"threshold_uncertainty_score":0.32054985},"labels":[],"label_agreement":null},{"id":"W1976406012","doi":"10.1088/0004-637x/691/2/1035","title":"FURTHER CONSTRAINTS ON THERMAL QUIESCENT X-RAY EMISSION FROM SAX J1808.4-3658","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":142,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Luminosity; Millisecond pulsar; Millisecond; Thermal; Pulsar; X-ray binary; X-ray burster","score_opus":0.012146868607874709,"score_gpt":0.23317368688646684,"score_spread":0.22102681827859214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976406012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966522,0.00019582288,0.0007658602,0.000063150124,0.000007278638,0.000006554652,0.00035252894,0.00006109768,0.0018956081],"genre_scores_gemma":[0.9978452,0.0000829991,0.0007576938,0.000079128455,0.00001983028,0.000008847885,0.00088215014,0.000027673872,0.00029645552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998523,0.000020283725,0.000013328323,0.00003830309,0.000033595872,0.000042178224],"domain_scores_gemma":[0.99939823,0.00016647448,0.00016561635,0.00007203008,0.00007317318,0.00012452947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040706366,0.0005693699,0.00056399725,0.00072834606,0.00043551886,0.0009352936,0.00050027843,0.00042022293,0.002905211],"category_scores_gemma":[0.0010975652,0.00036680192,0.00040436102,0.0005425874,0.0003338458,0.00046282346,0.0007376373,0.0004299298,0.00044523008],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007334746,0.00023557869,0.7802405,0.00019314542,0.00019415542,0.0011701903,0.0010399539,0.0053529437,0.19094828,0.004084942,0.0015158328,0.014291103],"study_design_scores_gemma":[0.00018343443,0.00028554845,0.9570207,0.00005858266,0.00015571204,0.0008281631,0.00059672346,0.018473767,0.009510267,0.0034740178,0.009347001,0.000066115485],"about_ca_topic_score_codex":0.002375289,"about_ca_topic_score_gemma":0.0055099325,"teacher_disagreement_score":0.002905211,"about_ca_system_score_codex":0.0004921199,"about_ca_system_score_gemma":0.00022909482,"threshold_uncertainty_score":0.009718955},"labels":[],"label_agreement":null},{"id":"W1976474231","doi":"10.1088/0004-637x/692/2/1506","title":"COOL WHITE DWARFS IDENTIFIED IN THE SECOND DATA RELEASE OF THE UKIRT INFRARED DEEP SKY SURVEY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Photometry (optics); Spectrograph; Sky; Massive compact halo object; Astrometry","score_opus":0.021820680173688364,"score_gpt":0.2479731342895092,"score_spread":0.22615245411582086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976474231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98562324,0.00016935325,0.0012902565,0.000049779366,0.00003157977,0.000050590526,0.009374122,0.00012003493,0.0032910376],"genre_scores_gemma":[0.9559992,0.000096391785,0.0028655652,0.00012943304,0.000025276815,0.00010065731,0.034772124,0.000058771646,0.0059525175],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990909,0.00006470948,0.00007038188,0.00018996531,0.0002891922,0.00029482116],"domain_scores_gemma":[0.9974558,0.00017051285,0.0008362089,0.0004159217,0.0005963761,0.00052506884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009395718,0.00031817303,0.0004496269,0.002502618,0.0005680164,0.0007057038,0.00045480923,0.00022754853,0.002589873],"category_scores_gemma":[0.0017089287,0.00017204533,0.00034150726,0.0015212912,0.00022691718,0.00028564836,0.0011664862,0.00027632355,0.0012839277],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036754028,0.000045635923,0.9663597,0.00007049932,0.00004623485,0.00051742047,0.00092208426,0.00021900187,0.01690528,0.00032179162,0.0033570025,0.0108678965],"study_design_scores_gemma":[0.000011945007,0.00007013457,0.98554045,0.000015834119,0.00002001414,0.0002082546,0.00022061216,0.00017006959,0.0024379462,0.000037404963,0.011255396,0.000011905418],"about_ca_topic_score_codex":0.034963425,"about_ca_topic_score_gemma":0.07617198,"teacher_disagreement_score":0.034963425,"about_ca_system_score_codex":0.000714401,"about_ca_system_score_gemma":0.0006003312,"threshold_uncertainty_score":0.06951982},"labels":[],"label_agreement":null},{"id":"W1976474330","doi":"10.1086/378947","title":"A New Distance Technique for Galactic Plane Objects","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Galactic plane; Astronomy; Astrophysics; Plane (geometry); Galaxy; Geometry","score_opus":0.006668285634027584,"score_gpt":0.2154889525392501,"score_spread":0.20882066690522252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976474330","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.047211993,0.0017698741,0.92269886,0.00019943334,0.00019389617,0.000104437866,0.0019477232,0.003441244,0.022432534],"genre_scores_gemma":[0.21068865,0.0008579253,0.77715045,0.00012280699,0.00015386887,0.0001799297,0.0024129883,0.00061199523,0.007821375],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99913603,0.0000661349,0.00005946935,0.00024508743,0.00042842745,0.00006488852],"domain_scores_gemma":[0.9985177,0.0002852637,0.0002589784,0.00040211176,0.0004263623,0.000109576205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004990082,0.0007300037,0.00053357915,0.0038589987,0.001025842,0.001748861,0.0015340501,0.0006108807,0.0052683484],"category_scores_gemma":[0.0026382492,0.00037467203,0.00054331427,0.0031129257,0.0006182666,0.0027355237,0.002173616,0.00096321554,0.002559433],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015279891,0.000059308048,0.07966849,0.00036561617,0.00017775972,0.00035725333,0.001108645,0.008338672,0.057704765,0.07349004,0.009288251,0.7692884],"study_design_scores_gemma":[0.00012315616,0.00044124655,0.15516509,0.00020279086,0.00024601625,0.007173524,0.0016273832,0.10950843,0.07879172,0.078317925,0.56793326,0.00046952738],"about_ca_topic_score_codex":0.010580149,"about_ca_topic_score_gemma":0.010975607,"teacher_disagreement_score":0.010580149,"about_ca_system_score_codex":0.00077000074,"about_ca_system_score_gemma":0.0006615707,"threshold_uncertainty_score":0.021037161},"labels":[],"label_agreement":null},{"id":"W1976518783","doi":"10.1086/382726","title":"Properties of Galaxy Dark Matter Halos from Weak Lensing","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":343,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Halo; Dark matter; Weak gravitational lensing; Dark matter halo; Galaxy; Velocity dispersion; Flattening; RADIUS; Cold dark matter","score_opus":0.009764476568045286,"score_gpt":0.19326071841844214,"score_spread":0.18349624185039687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976518783","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980484,0.00012886421,0.0008654674,0.00001505414,0.0000010644583,0.0000041873186,0.00029269548,0.000036641217,0.0006076318],"genre_scores_gemma":[0.9987005,0.00005739239,0.0002443126,0.000004596054,0.0000047703015,0.0000023070706,0.00089435576,0.000011967996,0.00007975191],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999729,0.000051465897,0.00001900396,0.00004016521,0.000083590465,0.00007690396],"domain_scores_gemma":[0.99418205,0.0019482436,0.0015747277,0.0006983169,0.0006284322,0.00096818554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012324642,0.00059033924,0.00037755547,0.0025715258,0.00040238103,0.0010976619,0.00033513663,0.00021751934,0.0012110024],"category_scores_gemma":[0.0058277673,0.00029194955,0.0005807071,0.0010998249,0.00069891074,0.0005674306,0.0009865542,0.00027127512,0.00022795265],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037579922,0.00002336968,0.95326346,0.00007918061,0.00023378362,0.00042396763,0.0005090159,0.020313015,0.014775799,0.001650882,0.00030568376,0.008046025],"study_design_scores_gemma":[0.000014132097,0.00008323378,0.96438974,0.000017849521,0.00006941112,0.00037497148,0.00021575391,0.027801437,0.004500226,0.0018461213,0.000653108,0.000034009554],"about_ca_topic_score_codex":0.0035604613,"about_ca_topic_score_gemma":0.0022501904,"teacher_disagreement_score":0.0035604613,"about_ca_system_score_codex":0.00049423706,"about_ca_system_score_gemma":0.00020039735,"threshold_uncertainty_score":0.007079482},"labels":[],"label_agreement":null},{"id":"W1976535397","doi":"10.1088/0004-637x/777/2/170","title":"PHOTON RINGS AROUND KERR AND KERR-LIKE BLACK HOLES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Rotating black hole; Kerr metric; Black hole (networking); Spin-flip; Schwarzschild radius; Supermassive black hole; Spins; Photon; Binary black hole; Quantum mechanics; Gravitation; Galaxy; Condensed matter physics; Angular momentum; Gravitational wave","score_opus":0.011114417578359122,"score_gpt":0.2173988754103051,"score_spread":0.20628445783194596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976535397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8898098,0.0005354726,0.09096639,0.00014736189,0.000032907636,0.000049457492,0.00010278907,0.0002539664,0.01810185],"genre_scores_gemma":[0.99385035,0.00012185201,0.005185432,0.000011606654,0.000010090308,0.0000101328815,0.00001939527,0.000035376277,0.00075578975],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998017,0.000077893215,0.000006159424,0.000028550183,0.000052204687,0.000033459306],"domain_scores_gemma":[0.99895346,0.00034073385,0.0003695738,0.00013893636,0.00007660993,0.000120730045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005902641,0.0003383289,0.00026516177,0.00057998055,0.00034043292,0.00068093813,0.00069736317,0.0005639962,0.001748841],"category_scores_gemma":[0.003043762,0.00031894565,0.0003435636,0.00024839654,0.0010623074,0.0015548667,0.0006353129,0.00032829525,0.0002500551],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019371971,0.000050625757,0.015386978,0.00013268078,0.00004555221,0.0007844006,0.000531304,0.3839705,0.026588025,0.559827,0.0010840244,0.011405124],"study_design_scores_gemma":[0.000046607478,0.00008307636,0.014338573,0.000030017987,0.00002293406,0.0008767456,0.00023754212,0.8822291,0.008533134,0.09111578,0.0024199067,0.000066644956],"about_ca_topic_score_codex":0.0004525192,"about_ca_topic_score_gemma":0.0003163974,"teacher_disagreement_score":0.001748841,"about_ca_system_score_codex":0.0004391527,"about_ca_system_score_gemma":0.00018956407,"threshold_uncertainty_score":0.0058504343},"labels":[],"label_agreement":null},{"id":"W1976546114","doi":"10.1088/0004-637x/707/1/693","title":"UNDERSTANDING THE X-RAY FLARING FROM η CARINAE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astrophysics; Physics; Brightness; Power law; Astronomy","score_opus":0.03308777327653061,"score_gpt":0.23765094209917093,"score_spread":0.2045631688226403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976546114","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955778,0.00036987037,0.0012054794,0.00006691773,0.0000033098904,0.0000062620306,0.00010440232,0.000009962771,0.0026559678],"genre_scores_gemma":[0.9983563,0.00034608098,0.0006048724,0.000017603454,0.000014161739,0.0000033076008,0.00021497409,0.0000038294297,0.00043877028],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999547,0.0000034108753,0.0000027412095,0.000013178313,0.000011604205,0.000014423926],"domain_scores_gemma":[0.99984777,0.000034335593,0.00006723185,0.000013140372,0.0000148426825,0.00002258379],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009729884,0.00023546135,0.00016609406,0.0006132977,0.00027612183,0.0009374102,0.0001945974,0.0004286334,0.0008168307],"category_scores_gemma":[0.0006948135,0.0001377191,0.00013578284,0.00039300436,0.00023050232,0.00083631504,0.0005105209,0.00022667911,0.00016043472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024328433,0.00006278432,0.81056094,0.00019450074,0.00009653005,0.002029721,0.002597675,0.028087212,0.08396377,0.0062365336,0.00053852156,0.06538854],"study_design_scores_gemma":[0.000002932348,0.000056288947,0.9815181,0.000016433434,0.000018688701,0.00071851205,0.00074373337,0.011521607,0.0015474001,0.0018883067,0.0019521926,0.000015821706],"about_ca_topic_score_codex":0.0036666652,"about_ca_topic_score_gemma":0.006267226,"teacher_disagreement_score":0.0036666652,"about_ca_system_score_codex":0.00019085921,"about_ca_system_score_gemma":0.00013683162,"threshold_uncertainty_score":0.0072906613},"labels":[],"label_agreement":null},{"id":"W1976613350","doi":"10.1086/339356","title":"On the Measurement of the Magnitude and Orientation of the Magnetic Field in Molecular Clouds","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Zeeman effect; Magnetic field; Polarimetry; Molecular cloud; Orientation (vector space); Line (geometry); Magnitude (astronomy); Field (mathematics)","score_opus":0.011579403078801337,"score_gpt":0.2104509112291327,"score_spread":0.19887150815033136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976613350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96549994,0.001009634,0.022885384,0.00008449523,0.000021561093,0.000033737888,0.00034135956,0.00016779701,0.009956246],"genre_scores_gemma":[0.98657423,0.000939444,0.011739657,0.000028666234,0.00003163358,0.000015455737,0.00012983961,0.000021762871,0.00051930104],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998908,0.000018620252,0.0000030814338,0.000017897994,0.00005024195,0.000019252553],"domain_scores_gemma":[0.99965894,0.00011693762,0.00008527651,0.00003749425,0.00007059875,0.000030783245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019771254,0.00020823702,0.00012959709,0.000786067,0.0002812991,0.00045021556,0.0002717675,0.00021614367,0.0006970948],"category_scores_gemma":[0.000740759,0.00014045065,0.000067851855,0.00062475156,0.00047034465,0.0003762216,0.00042969198,0.00022655813,0.00037524878],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042829098,0.00004302312,0.11395777,0.00016113056,0.000033944107,0.00044900004,0.00021519726,0.0034179483,0.7834081,0.004392013,0.0004167457,0.09307688],"study_design_scores_gemma":[0.000056469642,0.00036629112,0.38387236,0.00007897312,0.000089970126,0.00206737,0.00028258906,0.020350268,0.58050936,0.0042105825,0.008046694,0.00006909561],"about_ca_topic_score_codex":0.0014285613,"about_ca_topic_score_gemma":0.0019087447,"teacher_disagreement_score":0.0014285613,"about_ca_system_score_codex":0.00013081357,"about_ca_system_score_gemma":0.00011877846,"threshold_uncertainty_score":0.0028404593},"labels":[],"label_agreement":null},{"id":"W1976645212","doi":"10.1088/0004-637x/700/2/1626","title":"THE PHOTOMETRIC AND KINEMATIC STRUCTURE OF FACE-ON DISK GALAXIES. II. INTEGRATED LINE PROFILE CHARACTERIZATION AND THE ORIGIN OF LINE PROFILE ASYMMETRY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Asymmetry; Astrophysics; Line (geometry); Kurtosis; Galaxy; Gaussian; Moment (physics); Computational physics; Geometry; Classical mechanics; Quantum mechanics","score_opus":0.005512370940087262,"score_gpt":0.2171463113790348,"score_spread":0.21163394043894754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976645212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974439,0.00005628322,0.0005988653,0.000007721283,7.1200714e-7,0.0000049026416,0.00027859732,0.000016038988,0.0015929706],"genre_scores_gemma":[0.9985868,0.000026216143,0.00066178455,0.0000035172814,0.0000019231618,0.0000023549724,0.00043271924,0.0000051740494,0.00027957725],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990034,0.000009991981,0.0000053102694,0.000029210467,0.000024566829,0.000030584586],"domain_scores_gemma":[0.99959403,0.000047733793,0.00016408939,0.0000508884,0.00007257145,0.0000707595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012275673,0.00019951367,0.0001355399,0.0015809083,0.00024040208,0.0006509024,0.0003001341,0.00020674965,0.0010992561],"category_scores_gemma":[0.0006247292,0.00009555086,0.00013948623,0.0007955017,0.00026276064,0.00034437093,0.000497031,0.00014704496,0.00048958056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000976258,0.000037431128,0.9498166,0.000018058063,0.000016929134,0.00014945702,0.00046287154,0.0011135879,0.020440778,0.00071430794,0.00018614386,0.026946269],"study_design_scores_gemma":[9.016213e-7,0.000016849317,0.9967362,0.000002286729,0.0000035372154,0.0001249243,0.00015337784,0.0014846593,0.0010649974,0.00017352428,0.00023587576,0.000002844239],"about_ca_topic_score_codex":0.004661462,"about_ca_topic_score_gemma":0.0077857547,"teacher_disagreement_score":0.004661462,"about_ca_system_score_codex":0.0005084702,"about_ca_system_score_gemma":0.00011705723,"threshold_uncertainty_score":0.009268701},"labels":[],"label_agreement":null},{"id":"W1976658296","doi":"10.1088/0004-637x/761/2/100","title":"X-RAY EMISSION FROM SN 2004dj: A TALE OF TWO SHOCKS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Supernova; Ejecta; Particle acceleration; Compton scattering; Electron; Cassiopeia A; Magnetic field; Supernova remnant","score_opus":0.011319315933242083,"score_gpt":0.24635970795701237,"score_spread":0.23504039202377028,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976658296","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99887604,0.00009350259,0.00015194812,0.000006354823,0.0000021788965,0.000004070765,0.00030772795,0.000022188828,0.0005361064],"genre_scores_gemma":[0.9972832,0.000078090714,0.0004593968,0.000010245119,0.000004907067,0.0000055160217,0.0014587964,0.0000065989434,0.00069327303],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999175,0.000006718978,0.000007791089,0.000019737818,0.000026654889,0.000021538408],"domain_scores_gemma":[0.9998084,0.00002351394,0.00006934384,0.000020452795,0.000031903717,0.000046318724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014842932,0.00026534233,0.00025969424,0.0013363805,0.00027360168,0.0006964015,0.00026978945,0.00022040661,0.0008591409],"category_scores_gemma":[0.0003429559,0.0001656643,0.00026182138,0.0006689519,0.0001761892,0.00018174775,0.0004497568,0.00022182167,0.00022932647],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052472466,0.00010830835,0.9262684,0.00008248337,0.00009225954,0.000690236,0.00026154405,0.00043437027,0.0570129,0.00028218958,0.0005681691,0.013674326],"study_design_scores_gemma":[0.000007682024,0.00006119574,0.9933344,0.000005139198,0.000017846905,0.00061737135,0.00009877984,0.00042637865,0.0045346157,0.00004533603,0.00084753276,0.0000037683496],"about_ca_topic_score_codex":0.0040606004,"about_ca_topic_score_gemma":0.0065511093,"teacher_disagreement_score":0.0040606004,"about_ca_system_score_codex":0.00044282273,"about_ca_system_score_gemma":0.00016887514,"threshold_uncertainty_score":0.008073926},"labels":[],"label_agreement":null},{"id":"W1976710234","doi":"10.1086/529582","title":"Overcoming the Circular Problem for Gamma‐Ray Bursts in Cosmological Global‐Fitting Analysis","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"","keywords":"CMB cold spot; Dark energy; Redshift; Observable; Lambda-CDM model; Markov chain Monte Carlo; Observational cosmology; Cosmological constant","score_opus":0.018751334245305264,"score_gpt":0.24965613558167768,"score_spread":0.23090480133637242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976710234","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.095591195,0.00034375716,0.9015118,0.0002540645,0.000026052949,0.000040934345,0.00015528001,0.0007380141,0.0013388545],"genre_scores_gemma":[0.5770811,0.00029442034,0.41862258,0.00023700652,0.000054400774,0.00016291207,0.0011125691,0.0011037526,0.0013312534],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9979032,0.0011301389,0.00014275774,0.0004196023,0.00029104916,0.000113183065],"domain_scores_gemma":[0.98992246,0.005706271,0.00069118885,0.0028245628,0.0006818631,0.00017364766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007979973,0.0009716595,0.0008505098,0.001936468,0.0014289423,0.0016136304,0.0013450031,0.0006990903,0.0016620805],"category_scores_gemma":[0.028167237,0.00063655904,0.0014556998,0.0024251472,0.0011096314,0.0015338222,0.002219226,0.0017537962,0.00034411182],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003843836,0.00016093419,0.15913413,0.00026637438,0.0013363217,0.00068327144,0.002213356,0.41596046,0.009341211,0.09992174,0.0041274424,0.3064703],"study_design_scores_gemma":[0.000030529118,0.000049235587,0.01598149,0.00006692063,0.00016446113,0.0002252808,0.0003282177,0.91073966,0.0040598838,0.06278262,0.00550102,0.00007063159],"about_ca_topic_score_codex":0.01104992,"about_ca_topic_score_gemma":0.014760915,"teacher_disagreement_score":0.01104992,"about_ca_system_score_codex":0.0007465453,"about_ca_system_score_gemma":0.001818312,"threshold_uncertainty_score":0.04220265},"labels":[],"label_agreement":null},{"id":"W1976807697","doi":"10.1088/0004-637x/695/1/552","title":"PHOTOIONIZED MIXING LAYER MODELS OF THE DIFFUSE IONIZED GAS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Opacity; Photoionization; Mixing (physics); Ionization; Line (geometry); Turbulence; Spectral line; Active galactic nucleus; Jet (fluid)","score_opus":0.011010430544355524,"score_gpt":0.2132346066387777,"score_spread":0.20222417609442217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976807697","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8789263,0.000606809,0.09861612,0.00042268392,0.00005437801,0.00013806311,0.00094396406,0.0005739692,0.019717695],"genre_scores_gemma":[0.98608947,0.00025526594,0.0070515852,0.00007055722,0.00002827371,0.000112121765,0.00035013468,0.00006319866,0.005979306],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999033,0.000020707323,0.0000048605116,0.000024478759,0.000016255084,0.000030397354],"domain_scores_gemma":[0.99973184,0.000054974837,0.00009142959,0.000035698034,0.000024750427,0.00006131401],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027388535,0.00082595256,0.00034796825,0.00045662635,0.00032425128,0.0011037482,0.0016360461,0.00071584684,0.001981121],"category_scores_gemma":[0.0009880578,0.00032204235,0.00085209357,0.0003954355,0.00065385073,0.0011220542,0.00073770405,0.00045736495,0.00061792135],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002546522,0.000089398396,0.011928823,0.000069361966,0.00009160722,0.00022582027,0.00028427204,0.91478735,0.011976783,0.05407097,0.00080782676,0.005413196],"study_design_scores_gemma":[0.0000836677,0.000057663776,0.0021487952,0.0000055280802,0.000023810842,0.0000622233,0.000029247421,0.9833171,0.00092242466,0.012445722,0.00088577974,0.00001809993],"about_ca_topic_score_codex":0.005649736,"about_ca_topic_score_gemma":0.0018047867,"teacher_disagreement_score":0.005649736,"about_ca_system_score_codex":0.00077456975,"about_ca_system_score_gemma":0.0003362545,"threshold_uncertainty_score":0.011233747},"labels":[],"label_agreement":null},{"id":"W1976833992","doi":"10.1088/0004-637x/787/1/16","title":"THE PHYSICAL CHARACTERISTICS OF THE GAS IN THE DISK OF CENTAURUS A USING THE<i>HERSCHEL SPACE OBSERVATORY</i>","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Centaurus A; Galaxy; Spiral galaxy; Hydrogen line; Line (geometry); Dust lane; Emission spectrum; Elliptical galaxy; Barred spiral galaxy","score_opus":0.01074206580588983,"score_gpt":0.2204917487626433,"score_spread":0.20974968295675347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976833992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99778074,0.0003834418,0.000119737655,0.000019894043,0.0000027983256,0.0000032985924,0.0004107534,0.000028583047,0.0012506465],"genre_scores_gemma":[0.99906117,0.00013256933,0.00029925717,0.000011141712,0.000011315894,0.0000024832464,0.0003687709,0.000004115163,0.000109256325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985313,0.000018183513,0.000010372012,0.000053196265,0.00003320199,0.0000318001],"domain_scores_gemma":[0.999471,0.000062631356,0.0002504454,0.000060079386,0.000048119044,0.00010776023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022786464,0.00027153594,0.00018382909,0.0017000774,0.00036861846,0.00079360994,0.000322415,0.0002447335,0.0009300245],"category_scores_gemma":[0.00062789617,0.00014646703,0.00017028188,0.00087636325,0.0003707722,0.0004804039,0.00055125967,0.00015891372,0.00033963207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014842863,0.000049004397,0.92679715,0.0000880248,0.00012804211,0.00019724679,0.00048451705,0.0011013558,0.05754732,0.00038917077,0.00046109513,0.012608718],"study_design_scores_gemma":[0.0000030974008,0.000026733356,0.9976489,0.000005684276,0.000014175369,0.0000748431,0.00008456,0.0005183207,0.0010112157,0.000074019415,0.0005324047,0.000006053651],"about_ca_topic_score_codex":0.0057230084,"about_ca_topic_score_gemma":0.007383792,"teacher_disagreement_score":0.0057230084,"about_ca_system_score_codex":0.00051913015,"about_ca_system_score_gemma":0.00013473725,"threshold_uncertainty_score":0.011379361},"labels":[],"label_agreement":null},{"id":"W1976865423","doi":"10.1086/338769","title":"Procyon B: Outside the Iron Box","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Astrophysics; Stars; Spectrograph; RADIUS; Spitzer Space Telescope; Astronomy; Degeneracy (biology); Spectral line","score_opus":0.013583232679795039,"score_gpt":0.21351616237630364,"score_spread":0.1999329296965086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976865423","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8968606,0.0010638041,0.0013190295,0.0009912829,0.0000530729,0.000014078081,0.00043799053,0.00026723926,0.09899297],"genre_scores_gemma":[0.98464084,0.00024231132,0.0010532232,0.0003485844,0.000023369139,0.0000053441117,0.000354438,0.00008189047,0.0132499905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991083,0.0000056908543,0.000002064356,0.000033760774,0.000015996982,0.000031715255],"domain_scores_gemma":[0.99966025,0.000026076397,0.000087305896,0.00004101407,0.000032084306,0.00015320879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001018522,0.00020178262,0.00023304384,0.00034639146,0.0011552734,0.00073566043,0.00026962024,0.00030161653,0.010650476],"category_scores_gemma":[0.00039113464,0.000078495505,0.000084898835,0.0003166832,0.0006311947,0.0006630398,0.001071866,0.00047350215,0.0016970073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020199462,0.00021414984,0.48038852,0.00069118006,0.00008588886,0.012987839,0.007014465,0.00106897,0.07292744,0.10437308,0.049716376,0.26851204],"study_design_scores_gemma":[0.00009075874,0.0003747856,0.62109745,0.00024516252,0.000047324098,0.02092541,0.0049206563,0.0009893312,0.009434819,0.024582097,0.3172498,0.00004231188],"about_ca_topic_score_codex":0.0055222106,"about_ca_topic_score_gemma":0.008016751,"teacher_disagreement_score":0.010650476,"about_ca_system_score_codex":0.00032219157,"about_ca_system_score_gemma":0.00034152335,"threshold_uncertainty_score":0.03562945},"labels":[],"label_agreement":null},{"id":"W1976893351","doi":"10.1088/0004-637x/750/1/2","title":"CRITICAL EVALUATION OF MAGNETIC FIELD DETECTIONS REPORTED FOR PULSATING B-TYPE STARS IN LIGHT OF ESPaDOnS, NARVAL, AND REANALYZED FORS1/2 OBSERVATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Royal Military College of Canada; Queen's University","funders":"","keywords":"Stars; Astrophysics; Physics; Magnetic field; Field (mathematics); Spectral line; Population; Astronomy","score_opus":0.049628581128872806,"score_gpt":0.30861646152901,"score_spread":0.2589878804001372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1976893351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93648785,0.0045335023,0.0049858517,0.009122979,0.0037351102,0.00076266716,0.010503444,0.00050537434,0.029363172],"genre_scores_gemma":[0.98073363,0.0011415436,0.0049333335,0.002098403,0.0010820809,0.0001178185,0.0025072359,0.00016371244,0.0072222156],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99530137,0.0009891189,0.0014370144,0.0005615517,0.001377131,0.0003338335],"domain_scores_gemma":[0.92922187,0.020666314,0.008728414,0.003563841,0.036100492,0.001719107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010586324,0.00044341644,0.0003448037,0.00639528,0.0012074175,0.0017912767,0.0013254237,0.000934996,0.0033328654],"category_scores_gemma":[0.04910972,0.00023288725,0.00042487856,0.002782662,0.001021708,0.0012213716,0.00077481306,0.0007113883,0.0007521069],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002237312,0.000075131094,0.88841546,0.00085025263,0.000210118,0.0021219891,0.0030568095,0.0003851357,0.020267263,0.0012489838,0.01872918,0.06240234],"study_design_scores_gemma":[0.000052793366,0.00024118746,0.95140344,0.00027987815,0.00016849485,0.0012616714,0.0035076393,0.0005356405,0.008207642,0.0003851545,0.033916358,0.000040038518],"about_ca_topic_score_codex":0.017093567,"about_ca_topic_score_gemma":0.029060388,"teacher_disagreement_score":0.017093567,"about_ca_system_score_codex":0.0015124471,"about_ca_system_score_gemma":0.0015774928,"threshold_uncertainty_score":0.055986464},"labels":[],"label_agreement":null},{"id":"W1977004877","doi":"10.1086/308217","title":"An Investigation of Gravitational Lensing in the Southern BL Lac PKS 0537−441","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Gravitational microlensing; Quasar; Redshift; Galaxy; Gravitational lens; Photometry (optics); Active galactic nucleus; BL Lac object","score_opus":0.009483514151690442,"score_gpt":0.2179041537678279,"score_spread":0.20842063961613747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977004877","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987109,0.00016417097,0.00008587235,0.000031340256,0.000001544323,0.000004499312,0.00007387814,0.000007409902,0.00092045293],"genre_scores_gemma":[0.9992023,0.00010625258,0.00016458417,0.000016177335,0.000007552346,0.0000015427595,0.00017223303,0.0000015042071,0.0003278855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998851,0.000016490338,0.000004978504,0.00002269994,0.000035743025,0.000034955454],"domain_scores_gemma":[0.99971265,0.00004468484,0.00009934549,0.000015984631,0.000035457673,0.00009181387],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002110947,0.00027103754,0.0002684726,0.0015179586,0.00058166956,0.00039006118,0.00015610718,0.00019291588,0.0014361187],"category_scores_gemma":[0.0004073024,0.00012887003,0.00020853784,0.0013318318,0.0003092566,0.00024138004,0.00039843272,0.00017970454,0.00025321046],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018640596,0.00009813242,0.95995694,0.000048545262,0.000075832155,0.002706704,0.0010598756,0.00035846035,0.019604634,0.00069615146,0.00038505788,0.0148232],"study_design_scores_gemma":[0.0000033887043,0.00008720435,0.9972186,0.0000027642348,0.000009600327,0.00074568857,0.00037492355,0.00034259693,0.00046227325,0.00011285609,0.0006361458,0.0000039900638],"about_ca_topic_score_codex":0.024175353,"about_ca_topic_score_gemma":0.027340777,"teacher_disagreement_score":0.024175353,"about_ca_system_score_codex":0.00060412096,"about_ca_system_score_gemma":0.00041315463,"threshold_uncertainty_score":0.04806924},"labels":[],"label_agreement":null},{"id":"W1977025171","doi":"10.1088/0004-637x/720/1/603","title":"OBSERVATIONAL DETERMINATION OF THE TURBULENT AMBIPOLAR DIFFUSION SCALE AND MAGNETIC FIELD STRENGTH IN MOLECULAR CLOUDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Western University","funders":"","keywords":"Ambipolar diffusion; Turbulence; Diffusion; Turbulent diffusion; Magnetic field; Molecular cloud; Scale (ratio); Dissipation; Field (mathematics)","score_opus":0.006285904363634846,"score_gpt":0.2213415896286596,"score_spread":0.21505568526502475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977025171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994985,0.00003171376,0.000099070865,0.000013847422,6.801629e-7,0.0000012997322,0.000080621656,0.0000027029544,0.00027150684],"genre_scores_gemma":[0.9997992,0.000022514676,0.00006243148,0.0000024249825,0.0000022037516,6.250898e-7,0.00009483056,7.7743397e-7,0.000015127145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986863,0.000027259908,0.0000136117615,0.000042007865,0.000022636486,0.000025833442],"domain_scores_gemma":[0.9983505,0.0003344439,0.00073308527,0.00016866655,0.00015970824,0.00025356043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002649937,0.00015755341,0.00014123307,0.0007272866,0.00025685653,0.00048740814,0.00020470278,0.00025433456,0.0003084066],"category_scores_gemma":[0.0015127741,0.0001852005,0.00012736167,0.0005538268,0.00047381298,0.0003419588,0.00045086324,0.000204701,0.00009545523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008744211,0.00003066066,0.98409134,0.000012935973,0.000041923064,0.000070694085,0.00016918196,0.001360817,0.011863072,0.0004011398,0.000044708446,0.0018260871],"study_design_scores_gemma":[0.0000062377426,0.000015688714,0.9973464,0.0000023562636,0.000009746306,0.00005354062,0.000049981456,0.001489223,0.0007940731,0.00009164478,0.00013552373,0.000005584027],"about_ca_topic_score_codex":0.004670854,"about_ca_topic_score_gemma":0.005948145,"teacher_disagreement_score":0.004670854,"about_ca_system_score_codex":0.00028704014,"about_ca_system_score_gemma":0.00011574825,"threshold_uncertainty_score":0.009287357},"labels":[],"label_agreement":null},{"id":"W1977050387","doi":"10.1086/507417","title":"A Reverberation‐based Mass for the Central Black Hole in NGC 4151","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":211,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Black hole (networking); Astrophysics; Reverberation mapping; Supermassive black hole; Galaxy; Normalization (sociology); Active galactic nucleus; Velocity dispersion; Reverberation; Astronomy","score_opus":0.012152783545877139,"score_gpt":0.22823290439446678,"score_spread":0.21608012084858963,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977050387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998836,0.000081196406,0.00037496068,0.0000124948865,0.000004806319,0.00000565504,0.00014299394,0.00004085328,0.000501178],"genre_scores_gemma":[0.9988336,0.000027412127,0.0006225667,0.0000064047285,0.000005175254,0.00000404905,0.00026699773,0.0000065274953,0.00022733353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998784,0.000012046343,0.000005439357,0.00005419916,0.000027905564,0.00002190333],"domain_scores_gemma":[0.9995608,0.000039796265,0.00018149761,0.00007126941,0.00006499112,0.0000817372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028883794,0.00037198976,0.0001851756,0.0013669865,0.0003661219,0.0005405878,0.00042309368,0.00024825754,0.0013616217],"category_scores_gemma":[0.0006964519,0.00016644823,0.00020127592,0.0002987176,0.00020950781,0.0003970679,0.0004812397,0.00022157034,0.0004787],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028982747,0.000060848088,0.90221447,0.000047025947,0.00007025769,0.0005086686,0.0009984612,0.00093389506,0.06718203,0.00024370846,0.0004461591,0.027004732],"study_design_scores_gemma":[0.000008157397,0.000049454688,0.993174,0.000006792129,0.00002038666,0.0001728718,0.00011679279,0.0016474335,0.004073263,0.00008172867,0.00064089004,0.000008307617],"about_ca_topic_score_codex":0.0074468777,"about_ca_topic_score_gemma":0.011884074,"teacher_disagreement_score":0.0074468777,"about_ca_system_score_codex":0.00047561375,"about_ca_system_score_gemma":0.000104636536,"threshold_uncertainty_score":0.014807105},"labels":[],"label_agreement":null},{"id":"W1977408941","doi":"10.1088/0004-637x/788/2/140","title":"THE EFFECTS OF THE LOCAL ENVIRONMENT ON ACTIVE GALACTIC NUCLEI","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Astronomy; Galaxy; Luminous infrared galaxy; Galaxy group; Peculiar galaxy; Radio galaxy; Extinction (optical mineralogy); Quasar; Redshift; Brightest cluster galaxy","score_opus":0.0026287318739468793,"score_gpt":0.17529080059136182,"score_spread":0.17266206871741493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977408941","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99539834,0.0009826196,0.00044493403,0.000121568555,0.0000092574965,0.0000042012307,0.0002529496,0.000011880425,0.0027742726],"genre_scores_gemma":[0.99954826,0.0001372346,0.000059915918,0.000016935603,0.000013646751,0.0000013443553,0.000084433756,0.0000068718273,0.00013129841],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99846244,0.0006162442,0.00007972423,0.0004169244,0.00024307413,0.00018161313],"domain_scores_gemma":[0.98964965,0.0041922643,0.0030802025,0.0013796955,0.00065526436,0.0010429142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010391981,0.0001827508,0.00041866655,0.0007760245,0.0005011227,0.0012538662,0.00053795817,0.00030069833,0.003012193],"category_scores_gemma":[0.008285652,0.00015874456,0.00040342423,0.0009919693,0.0013222906,0.0010707378,0.0010560494,0.00027108664,0.0005774827],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009188467,0.00001393374,0.9912976,0.00002743435,0.00015315038,0.00009731443,0.00017275893,0.0002740586,0.0011733129,0.00034313597,0.00009240498,0.0062630805],"study_design_scores_gemma":[9.650241e-7,0.000025534942,0.99911696,0.0000050285503,0.000020641588,0.00006716419,0.00014912202,0.00014749212,0.00012573379,0.00010684289,0.00023193104,0.0000026009475],"about_ca_topic_score_codex":0.0034355365,"about_ca_topic_score_gemma":0.0049461317,"teacher_disagreement_score":0.0034355365,"about_ca_system_score_codex":0.0003006112,"about_ca_system_score_gemma":0.00018425728,"threshold_uncertainty_score":0.010076761},"labels":[],"label_agreement":null},{"id":"W1977410614","doi":"10.1086/376357","title":"Gravitational Collapse of Filamentary Magnetized Molecular Clouds","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Hydrostatic equilibrium; Gravitational collapse; Toroid; Magnetic field; Density contrast; Magnetohydrodynamics; Gravitational instability; Gravitation; Magnetization","score_opus":0.006757528946483193,"score_gpt":0.2314952740895404,"score_spread":0.22473774514305722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977410614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93485194,0.0005533003,0.049303252,0.00068379205,0.00004269932,0.000080240934,0.00014739057,0.00019697567,0.014140464],"genre_scores_gemma":[0.9925315,0.00023395251,0.0041385144,0.000060773553,0.000030324816,0.000041226212,0.00008635556,0.000023917266,0.0028535137],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999889,0.000029347964,0.000004643633,0.00001185912,0.000028166549,0.00003698883],"domain_scores_gemma":[0.9997192,0.000050955918,0.00008918079,0.000019349669,0.00004005305,0.00008129069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022948353,0.0005189696,0.00035328802,0.00052700273,0.0008922104,0.00074969535,0.0011471867,0.0010204527,0.00085741654],"category_scores_gemma":[0.0013965314,0.0003025981,0.0005842711,0.00029814942,0.00082493003,0.0007184268,0.0010493331,0.00037473952,0.00015246433],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052557087,0.000042756288,0.0038487543,0.000028230712,0.000046143752,0.0005735573,0.00018118531,0.9324844,0.003818783,0.05653325,0.000550953,0.0018394566],"study_design_scores_gemma":[0.00002181982,0.00001747416,0.0009633643,0.000004562156,0.0000065688027,0.00006667708,0.000031077885,0.99249905,0.00029331847,0.0055099297,0.0005779541,0.000008172559],"about_ca_topic_score_codex":0.029230088,"about_ca_topic_score_gemma":0.013824218,"teacher_disagreement_score":0.029230088,"about_ca_system_score_codex":0.0016792478,"about_ca_system_score_gemma":0.0006513852,"threshold_uncertainty_score":0.058119893},"labels":[],"label_agreement":null},{"id":"W1977444383","doi":"10.1086/586692","title":"Ultraviolet Observations of the X‐Ray Photoionized Wind of Cygnus X‐1 during X‐Ray Soft/High State1","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"RADIUS; Photoionization; Luminosity; Accretion (finance); Ultraviolet; Line (geometry); Binary number; Black hole (networking)","score_opus":0.01664728480567242,"score_gpt":0.21257673118643514,"score_spread":0.1959294463807627,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977444383","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993579,0.000024998026,0.0000821872,0.000005562812,0.0000010196835,0.000002523409,0.00015388924,0.000007510151,0.0003642631],"genre_scores_gemma":[0.9988951,0.00003654508,0.00030187756,0.0000052065734,0.0000029036787,0.00000388808,0.0004589002,0.000003033543,0.00029258503],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999747,0.0000037241641,0.0000016288577,0.0000061691153,0.0000071640975,0.000006537633],"domain_scores_gemma":[0.9999045,0.000012412736,0.000028698927,0.0000067018555,0.00001307176,0.000034513872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012789934,0.00013232722,0.00009446946,0.00029802296,0.00020503523,0.00018370434,0.000115344985,0.00013734141,0.0009797683],"category_scores_gemma":[0.00022174344,0.00009667172,0.00008006204,0.00015859432,0.000076483484,0.00010195685,0.000202704,0.00024076749,0.00022703255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048831955,0.00013261457,0.84652334,0.00005219467,0.00005757118,0.00048661322,0.0005878112,0.0034470556,0.1328025,0.00033817455,0.0006271484,0.014456522],"study_design_scores_gemma":[0.000004258883,0.000052530166,0.99710435,0.0000030781262,0.0000041860076,0.000059112983,0.000029913095,0.001518982,0.0009067419,0.000022364935,0.0002922491,0.0000022182223],"about_ca_topic_score_codex":0.0033424431,"about_ca_topic_score_gemma":0.008067618,"teacher_disagreement_score":0.0033424431,"about_ca_system_score_codex":0.00019907983,"about_ca_system_score_gemma":0.00006126182,"threshold_uncertainty_score":0.0066459775},"labels":[],"label_agreement":null},{"id":"W1977473941","doi":"10.1088/0004-637x/747/2/96","title":"A STUDY OF THE DARK CORE IN A520 WITH THE<i>HUBBLE SPACE TELESCOPE</i>: THE MYSTERY DEEPENS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Dark matter; Galaxy; Astronomy; Luminosity; Weak gravitational lensing; Advanced Camera for Surveys; Galaxy cluster; Hubble space telescope; Redshift","score_opus":0.011325805295017928,"score_gpt":0.21701807272313736,"score_spread":0.20569226742811944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977473941","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983693,0.00013126568,0.00013663419,0.000041853407,0.0000030748145,0.000005972491,0.00018017595,0.0000071826585,0.0011245934],"genre_scores_gemma":[0.9981238,0.00009640511,0.00045380267,0.000057341855,0.000014602377,0.0000029022506,0.0005298061,0.0000057202274,0.00071548927],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992704,0.000008046503,0.0000030282813,0.000018471015,0.000012390284,0.000031090054],"domain_scores_gemma":[0.99973875,0.000015256546,0.000065970504,0.000017751827,0.00003410053,0.00012806182],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021281652,0.0002943374,0.0001731316,0.0011013693,0.0008583995,0.00051160326,0.0003265276,0.00033899705,0.0011794958],"category_scores_gemma":[0.00022258416,0.00018996595,0.00021842484,0.0007422404,0.0003657031,0.0003440316,0.00067899923,0.00024237817,0.00050206576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002879204,0.00017609421,0.94,0.00003883176,0.000053141146,0.0023000827,0.0016104438,0.00028613978,0.042792678,0.0006606299,0.001071547,0.010722346],"study_design_scores_gemma":[0.000002567976,0.000066553526,0.99781394,0.0000042827837,0.0000073354145,0.00038856704,0.00029725675,0.00017646227,0.00035515754,0.000053906202,0.0008301348,0.000003833911],"about_ca_topic_score_codex":0.023414781,"about_ca_topic_score_gemma":0.041108273,"teacher_disagreement_score":0.023414781,"about_ca_system_score_codex":0.0004984278,"about_ca_system_score_gemma":0.0001915847,"threshold_uncertainty_score":0.04655701},"labels":[],"label_agreement":null},{"id":"W1977616389","doi":"10.1088/0004-637x/719/1/28","title":"A MODEL OF MAGNETIC BRAKING OF SOLAR ROTATION THAT SATISFIES OBSERVATIONAL CONSTRAINTS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Tachocline; Magnetic diffusivity; Radiative transfer; Solar rotation; Angular momentum; Magnetic field; Magnetohydrodynamics; Rotation (mathematics); Turbulence; Convection zone","score_opus":0.024382081989517405,"score_gpt":0.2419474070416634,"score_spread":0.21756532505214599,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977616389","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34579954,0.001374501,0.51252615,0.003393579,0.0008091541,0.00025999144,0.0018230032,0.00080894196,0.13320516],"genre_scores_gemma":[0.92763406,0.00067497516,0.030751618,0.00036720626,0.0002495775,0.0003742317,0.00053052214,0.0001393064,0.039278552],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998258,0.000048172406,0.000008762161,0.000045507484,0.000035846726,0.00003589736],"domain_scores_gemma":[0.9997414,0.000063104795,0.000049451715,0.000032594908,0.000049755698,0.000063800755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002592287,0.000628669,0.0011524666,0.00044150226,0.00086785207,0.0015501914,0.0024034155,0.0027471557,0.004299982],"category_scores_gemma":[0.00083526305,0.0005000443,0.0009251694,0.00066276686,0.0011875362,0.0012725537,0.0011499708,0.0010977936,0.001036767],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014359123,0.00007605032,0.00091377256,0.000101992075,0.000041030646,0.00051738403,0.0002092113,0.865089,0.005738568,0.12147963,0.0016243854,0.0040653595],"study_design_scores_gemma":[0.000096983196,0.000038698297,0.00036803877,0.0000074771006,0.000012334782,0.00010323138,0.00003641941,0.98425215,0.00024055134,0.012946166,0.0018762264,0.000021642312],"about_ca_topic_score_codex":0.008437102,"about_ca_topic_score_gemma":0.0031851334,"teacher_disagreement_score":0.008437102,"about_ca_system_score_codex":0.0007149132,"about_ca_system_score_gemma":0.0009918875,"threshold_uncertainty_score":0.016775966},"labels":[],"label_agreement":null},{"id":"W1977737562","doi":"10.1086/431924","title":"The Emergence of the Thick Disk in a CDM Universe. II. Colors and Abundance Patterns","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Milky Way; Thick disk; Stars; Halo; Galaxy formation and evolution; Galaxy; Population; Abundance (ecology)","score_opus":0.004933183451055457,"score_gpt":0.20003136288600898,"score_spread":0.19509817943495353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977737562","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965593,0.00019628288,0.000637747,0.000057513942,0.0000016628994,0.000005556012,0.00011304508,0.000013602583,0.0024151348],"genre_scores_gemma":[0.99874735,0.000075480755,0.0006586506,0.000017803803,0.0000029426003,0.0000028374563,0.00008637001,0.0000050169583,0.00040349856],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999573,0.000010522417,0.0000019242848,0.000013233472,0.000006548476,0.000010488194],"domain_scores_gemma":[0.99971694,0.00005889341,0.000082286,0.000036062982,0.000038440827,0.00006732988],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015010194,0.00012439689,0.00010157722,0.0006032872,0.0003301952,0.0008396203,0.00025140675,0.00030656383,0.0010314363],"category_scores_gemma":[0.001098975,0.00015977613,0.00007849834,0.00037783023,0.0004888922,0.00057011464,0.0004341007,0.00028583797,0.0001448965],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006675898,0.000111740024,0.859242,0.000108248554,0.000051941195,0.001154115,0.0015703075,0.017486392,0.04493694,0.03435344,0.0017964321,0.03852083],"study_design_scores_gemma":[0.0000496077,0.000072504066,0.9239806,0.000035413825,0.00003215643,0.00093972887,0.0010330904,0.043246023,0.005061684,0.020945603,0.0045769406,0.00002667904],"about_ca_topic_score_codex":0.002212703,"about_ca_topic_score_gemma":0.0022641325,"teacher_disagreement_score":0.002212703,"about_ca_system_score_codex":0.00045869357,"about_ca_system_score_gemma":0.00006533872,"threshold_uncertainty_score":0.0043996572},"labels":[],"label_agreement":null},{"id":"W1977782769","doi":"10.1088/0004-637x/765/1/67","title":"THE ATACAMA COSMOLOGY TELESCOPE: PHYSICAL PROPERTIES OF SUNYAEV-ZEL'DOVICH EFFECT CLUSTERS ON THE CELESTIAL EQUATOR<sup>,</sup>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; ROSAT; Sky; Galaxy cluster; Telescope; Redshift; Galaxy; Astronomy; South Pole Telescope; Large Synoptic Survey Telescope; Cosmology; Observatory","score_opus":0.008188240145282072,"score_gpt":0.20439149216187302,"score_spread":0.19620325201659095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977782769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9686998,0.0003487603,0.00050758966,0.00009089752,0.000023519518,0.000026879865,0.021748684,0.00010342304,0.00845032],"genre_scores_gemma":[0.97211987,0.00017159429,0.0008591088,0.00003830496,0.000051130075,0.00001929801,0.024922667,0.000049622,0.0017684556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984014,0.000015224286,0.0000096221775,0.000035118006,0.000059772676,0.00004006806],"domain_scores_gemma":[0.9989749,0.00010726719,0.0003576439,0.00011371934,0.00014896948,0.00029748768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002542017,0.00020077394,0.0002350045,0.0015532781,0.00034405454,0.0004968712,0.00044429098,0.00016714995,0.005402717],"category_scores_gemma":[0.00073310465,0.00013699297,0.00016661464,0.0014408352,0.0002304942,0.00028823796,0.0004912007,0.00020527077,0.0014071447],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014742398,0.000024686835,0.9789848,0.000034702967,0.00003914704,0.00005621664,0.00020718186,0.0005411782,0.0034286503,0.00033055196,0.008720018,0.007485473],"study_design_scores_gemma":[0.0000019173353,0.000003102065,0.9983359,0.0000013637837,0.0000034050126,0.000021345662,0.000030713898,0.00011064763,0.00010445499,0.000017567021,0.0013683677,0.0000012528157],"about_ca_topic_score_codex":0.025459077,"about_ca_topic_score_gemma":0.028930359,"teacher_disagreement_score":0.025459077,"about_ca_system_score_codex":0.00039623733,"about_ca_system_score_gemma":0.00020204157,"threshold_uncertainty_score":0.050621808},"labels":[],"label_agreement":null},{"id":"W1977783347","doi":"10.1088/0004-637x/748/2/115","title":"KOI 1224: A FOURTH BLOATED HOT WHITE DWARF COMPANION FOUND WITH<i>KEPLER</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"White dwarf; Physics; Astrophysics; Orbital period; Light curve; Kepler; Astronomy; Effective temperature; Stars","score_opus":0.014436557089643013,"score_gpt":0.22253955045278742,"score_spread":0.20810299336314442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977783347","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98736763,0.00016751008,0.0020034714,0.000054836117,0.0000129729515,0.000029482168,0.00047288215,0.000099296136,0.00979199],"genre_scores_gemma":[0.9889999,0.00012069569,0.0048397603,0.000031978365,0.000012157603,0.000017312575,0.002302437,0.000052057014,0.003623776],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994123,0.000003827671,0.0000031173224,0.00001645601,0.000016312633,0.000019029685],"domain_scores_gemma":[0.99990094,0.00000878599,0.000042659132,0.000012486993,0.0000073632737,0.000027725888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000043562584,0.00036121573,0.00028655722,0.0009909676,0.00053976226,0.0006769087,0.00039580982,0.00038841343,0.0022735514],"category_scores_gemma":[0.00021662666,0.000134096,0.00025179726,0.0007423575,0.0003631131,0.00031078648,0.00085656025,0.00031867513,0.0008493496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015911106,0.00025636205,0.75243133,0.0004079015,0.00016783286,0.014082468,0.0017265356,0.015703894,0.10581847,0.013792305,0.0067801555,0.08724157],"study_design_scores_gemma":[0.000105054016,0.000650156,0.83700407,0.00006170079,0.00017662146,0.024426904,0.0015844516,0.03965308,0.023908114,0.0060885493,0.06622681,0.00011440967],"about_ca_topic_score_codex":0.0022456173,"about_ca_topic_score_gemma":0.0028936535,"teacher_disagreement_score":0.0022735514,"about_ca_system_score_codex":0.0005811008,"about_ca_system_score_gemma":0.00021917002,"threshold_uncertainty_score":0.007605791},"labels":[],"label_agreement":null},{"id":"W1977791429","doi":"10.1088/0004-637x/705/1/529","title":"DUST DISTRIBUTION IN THE β PICTORIS CIRCUMSTELLAR DISKS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planetesimal; Physics; Astrophysics; Circumstellar disk; RADIUS; Circumstellar dust; Hubble space telescope; Protoplanetary disk; Thick disk; Planetary system; Astronomy; Cosmic dust; Solar System; Stars","score_opus":0.010562148154797937,"score_gpt":0.24203235940443096,"score_spread":0.23147021124963302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1977791429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903639,0.0002598233,0.0041636205,0.00020551404,0.000009152046,0.000016965487,0.00033609127,0.00010630637,0.00453849],"genre_scores_gemma":[0.99877447,0.00011888619,0.0005756779,0.000025946572,0.0000067289593,0.000011432099,0.00008285074,0.000011078236,0.00039295823],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999243,0.000026901454,0.0000032894327,0.000020103307,0.000009643124,0.000015746527],"domain_scores_gemma":[0.9997733,0.00007512532,0.000058177542,0.000022881139,0.000023165254,0.00004742606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000184486,0.0005588884,0.00035042924,0.0005445744,0.00037717432,0.0012376768,0.0009951148,0.0008657294,0.00084098114],"category_scores_gemma":[0.00076371175,0.00042656678,0.0006223394,0.0004310647,0.00051311165,0.00049629394,0.00030159325,0.00037606314,0.0003014064],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022726328,0.00007508233,0.06856041,0.000031029467,0.0000774338,0.0007395556,0.00023402297,0.9197264,0.0035340867,0.0034944792,0.00072782044,0.0025725241],"study_design_scores_gemma":[0.00008638715,0.00007811897,0.03230989,0.000019188328,0.000027666763,0.00029062803,0.00009682553,0.96258956,0.00044215645,0.0032309103,0.00079408666,0.000034550096],"about_ca_topic_score_codex":0.01295639,"about_ca_topic_score_gemma":0.004423079,"teacher_disagreement_score":0.01295639,"about_ca_system_score_codex":0.0011592198,"about_ca_system_score_gemma":0.0002612172,"threshold_uncertainty_score":0.025761962},"labels":[],"label_agreement":null},{"id":"W1978010038","doi":"10.1088/0004-637x/753/1/47","title":"A<i>CHANDRA</i>-VLA INVESTIGATION OF THE X-RAY CAVITY SYSTEM AND RADIO MINI-HALO IN THE GALAXY CLUSTER RBS 797","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Università di Bologna; Smithsonian Institution","keywords":"Physics; Astrophysics; Halo; Galaxy; Cooling flow; Cluster (spacecraft); Metallicity; Galaxy cluster; Astronomy; Radio halo","score_opus":0.008328454042574499,"score_gpt":0.19791792781505782,"score_spread":0.1895894737724833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978010038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978065,0.00034945068,0.00017554767,0.000025514952,0.0000026476664,0.000005790121,0.000257337,0.000030865438,0.0013463488],"genre_scores_gemma":[0.9983045,0.000107397704,0.0006921439,0.000011359832,0.000009419213,0.0000043008476,0.0006174146,0.000010858541,0.00024267877],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.000006608539,0.000003105867,0.000021047208,0.000020847658,0.000031337702],"domain_scores_gemma":[0.999648,0.00003367098,0.00009469332,0.000039924158,0.00005099604,0.00013267098],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011124415,0.00019626346,0.00027759233,0.0017100225,0.0005220553,0.0005317149,0.00031647977,0.00016285438,0.00081481645],"category_scores_gemma":[0.0001989102,0.00011414612,0.0002593026,0.00095276843,0.00031732087,0.00019214925,0.0005768767,0.00018830699,0.00027167343],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060095306,0.00018541212,0.74538296,0.00015656865,0.0001792323,0.0026639982,0.0007430027,0.0027741583,0.21641643,0.0018537872,0.0017488615,0.027294604],"study_design_scores_gemma":[0.000012114005,0.0000791759,0.9914231,0.000007966948,0.000027120332,0.0006323978,0.00021755224,0.002406634,0.0033777968,0.00020185503,0.0015960488,0.00001836435],"about_ca_topic_score_codex":0.007717022,"about_ca_topic_score_gemma":0.009874968,"teacher_disagreement_score":0.007717022,"about_ca_system_score_codex":0.0003781772,"about_ca_system_score_gemma":0.00029723893,"threshold_uncertainty_score":0.0153442025},"labels":[],"label_agreement":null},{"id":"W1978043477","doi":"10.1088/0004-637x/735/1/62","title":"COOL WHITE DWARFS FOUND IN THE UKIRT INFRARED DEEP SKY SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Sky; White dwarf; Infrared; White (mutation); Astrophysics; Astronomy; Physics; Environmental science; Chemistry; Stars","score_opus":0.02751796384757523,"score_gpt":0.2332586642155944,"score_spread":0.20574070036801917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978043477","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964658,0.00023681938,0.0003037152,0.000019506193,0.000004305776,0.0000050134327,0.0017073622,0.000025317264,0.0012321399],"genre_scores_gemma":[0.994333,0.00011897474,0.00048133836,0.00003103097,0.000004818518,0.00000695363,0.0041006906,0.000011400359,0.0009118161],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962807,0.000025244919,0.00002285448,0.00009471338,0.000121638164,0.00010741699],"domain_scores_gemma":[0.9991161,0.00006587562,0.00035605335,0.00007950771,0.00016843311,0.00021403629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033719494,0.00019307285,0.00024689533,0.0014930591,0.000314174,0.00047349537,0.00026982647,0.00012584109,0.0010676343],"category_scores_gemma":[0.0007016413,0.00013381625,0.00019156131,0.0013992285,0.00021311136,0.00021690216,0.00082792493,0.00015201085,0.00050599454],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009907192,0.00001448438,0.9857734,0.00002408357,0.000029820749,0.00017560273,0.00049881905,0.00009697426,0.0069202413,0.00012973596,0.0008686465,0.005369133],"study_design_scores_gemma":[0.0000029400235,0.000018730989,0.99653,0.0000049947616,0.000010693379,0.0001252827,0.00013778379,0.000080818194,0.00042089383,0.000018128576,0.0026464192,0.0000033376236],"about_ca_topic_score_codex":0.026433619,"about_ca_topic_score_gemma":0.069079354,"teacher_disagreement_score":0.026433619,"about_ca_system_score_codex":0.0006030555,"about_ca_system_score_gemma":0.00024060317,"threshold_uncertainty_score":0.052559495},"labels":[],"label_agreement":null},{"id":"W1978113522","doi":"10.1086/529371","title":"Draping of Cluster Magnetic Fields over Bullets and Bubbles—Morphology and Dynamic Effects","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":247,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Magnetic field; L-shell; Magnetohydrodynamics; Slipping; Vorticity; Core (optical fiber); Turbulence; Plasma; Cluster (spacecraft); Field line","score_opus":0.004541665846847004,"score_gpt":0.21283869883787904,"score_spread":0.20829703299103203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978113522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984162,0.00007500953,0.000725851,0.000019557854,0.000001638443,0.0000024581543,0.000020458861,0.000047628833,0.00069130695],"genre_scores_gemma":[0.99940515,0.000018340728,0.0002877991,0.0000056096915,0.0000018944258,0.0000014901188,0.000022644212,0.000011019396,0.00024600571],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999461,0.0000045784896,0.0000016146445,0.0000148775325,0.000012128059,0.000020585125],"domain_scores_gemma":[0.99968195,0.00004564288,0.000098973076,0.000039578714,0.000039646908,0.00009407365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006856663,0.00013758273,0.00016527018,0.0003637154,0.00033284535,0.00054704136,0.00033573687,0.00021160675,0.0005525176],"category_scores_gemma":[0.00048344588,0.00021487729,0.00011927592,0.00015986436,0.00034711906,0.00024637044,0.00041673635,0.00018825369,0.00011410802],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007725431,0.00010401747,0.07217623,0.000079915364,0.00006402888,0.0015365933,0.0009109951,0.036770865,0.85283273,0.0036819677,0.00086300273,0.030207016],"study_design_scores_gemma":[0.000104775245,0.0005417173,0.57029957,0.000027500875,0.000073994765,0.0019612536,0.0007933769,0.26300034,0.15587896,0.0027624024,0.004442098,0.00011406256],"about_ca_topic_score_codex":0.0020583528,"about_ca_topic_score_gemma":0.0010755592,"teacher_disagreement_score":0.0020583528,"about_ca_system_score_codex":0.00049222226,"about_ca_system_score_gemma":0.00009669569,"threshold_uncertainty_score":0.0040926933},"labels":[],"label_agreement":null},{"id":"W1978175334","doi":"10.1088/0004-637x/709/2/611","title":"THE QUASAR OUTFLOW CONTRIBUTION TO AGN FEEDBACK: VLT MEASUREMENTS OF SDSS J0318-0600","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":214,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Quasar; Outflow; Photoionization; Luminosity; Lyman limit; Active galactic nucleus; Flux (metallurgy); Spectral line; Line (geometry)","score_opus":0.010279008652161099,"score_gpt":0.22709199586292003,"score_spread":0.21681298721075892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978175334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980317,0.000051187435,0.00027879846,0.000031980944,0.000005043791,0.0000064456344,0.00073009083,0.000053465625,0.0008112476],"genre_scores_gemma":[0.997426,0.00005061524,0.00075687974,0.000049600716,0.000013792128,0.0000134577895,0.0014779426,0.000014500499,0.00019728005],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998623,0.00001560744,0.000012988636,0.000037577665,0.000037402795,0.000034010067],"domain_scores_gemma":[0.99939096,0.00006547392,0.00019505006,0.000042725296,0.0000954061,0.00021035725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031016365,0.00028786174,0.00030512543,0.0010852923,0.00033791483,0.00073548453,0.0004803382,0.00042334705,0.00081982306],"category_scores_gemma":[0.0006371093,0.00020824475,0.00025332102,0.0007251809,0.00022325135,0.00028905034,0.00041826506,0.00036138966,0.00039431822],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019301126,0.0002515441,0.94664836,0.000034299712,0.00006897502,0.00037677138,0.00043995696,0.0008078734,0.04107022,0.00023972055,0.00089561613,0.008973637],"study_design_scores_gemma":[0.000023195471,0.000060602062,0.9937721,0.0000075001853,0.000029585492,0.0002450859,0.000115469025,0.0025427463,0.0022170718,0.00008375759,0.00089185266,0.000011042994],"about_ca_topic_score_codex":0.0073741074,"about_ca_topic_score_gemma":0.013989564,"teacher_disagreement_score":0.0073741074,"about_ca_system_score_codex":0.00049505604,"about_ca_system_score_gemma":0.0001743153,"threshold_uncertainty_score":0.014662385},"labels":[],"label_agreement":null},{"id":"W1978176599","doi":"10.1088/0004-637x/715/1/541","title":"SN 2007od: A TYPE IIP SUPERNOVA WITH CIRCUMSTELLAR INTERACTION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Ejecta; Astrophysics; Physics; Supernova; Flattening; Photometry (optics); Brightness; Torus; Circumstellar dust; Astronomy; Extinction (optical mineralogy); Surface brightness; Emission spectrum; Spectral line; Cosmic dust; Stars; Galaxy; Optics","score_opus":0.009665889844609024,"score_gpt":0.23356965535319552,"score_spread":0.22390376550858648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978176599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98523444,0.0005196439,0.0028154952,0.00019852725,0.00014606075,0.0001234639,0.0014663374,0.00019792459,0.00929815],"genre_scores_gemma":[0.98853636,0.0003210576,0.0026985195,0.00038975256,0.000096023694,0.00005054325,0.0042182025,0.000055209544,0.0036342207],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998311,0.0000107804135,0.000018762292,0.000052566633,0.00004238568,0.000044386186],"domain_scores_gemma":[0.99969673,0.000019716907,0.000070529066,0.00003566956,0.000030586874,0.00014678773],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018447156,0.00065323815,0.0004933484,0.0006642539,0.0006578803,0.0006050668,0.00028522193,0.0006108531,0.0016843764],"category_scores_gemma":[0.00029012185,0.00017935962,0.0006113936,0.000478567,0.00042857372,0.00020213619,0.0011205048,0.0005709749,0.00043276884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000755091,0.00037334007,0.86972433,0.00017890533,0.00039321225,0.04754059,0.00018457683,0.00055518805,0.035424683,0.0026244544,0.0072323666,0.035013296],"study_design_scores_gemma":[0.00013052675,0.0008190188,0.7648295,0.00008043921,0.00017949364,0.1804463,0.0003552202,0.002355262,0.010520493,0.0016696021,0.038574986,0.00003924828],"about_ca_topic_score_codex":0.0028612632,"about_ca_topic_score_gemma":0.006118882,"teacher_disagreement_score":0.0028612632,"about_ca_system_score_codex":0.00039516398,"about_ca_system_score_gemma":0.00040915987,"threshold_uncertainty_score":0.0056892037},"labels":[],"label_agreement":null},{"id":"W1978188911","doi":"10.1086/320245","title":"Trans‐Relativistic Blast Waves in Supernovae as Gamma‐Ray Burst Progenitors","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":181,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Ejecta; Supernova; Gamma-ray burst; Astrophysics; Blast wave; Radiative transfer; Relativistic speed; Kinetic energy; Shock wave; Luminosity; Particle acceleration; Acceleration; Astronomy; Nuclear physics; Relativistic particle; Classical mechanics; Mechanics; Electron; Quantum mechanics","score_opus":0.011191539266058294,"score_gpt":0.23506803695543943,"score_spread":0.22387649768938114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978188911","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88398963,0.0020827989,0.10118292,0.00028931597,0.000074976146,0.00004119048,0.000088265515,0.00017697274,0.01207403],"genre_scores_gemma":[0.9856792,0.0015711604,0.008637765,0.000031665495,0.00004883161,0.00003699421,0.00007290656,0.000042432275,0.0038789515],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999291,0.000026654003,0.0000031781158,0.000009120337,0.000016850161,0.000015075101],"domain_scores_gemma":[0.99983823,0.00004052916,0.00004915866,0.0000165405,0.000026341155,0.00002923156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027637178,0.0005661273,0.00039985141,0.00040327947,0.00034603383,0.00097325764,0.0006048065,0.00053741544,0.00060816924],"category_scores_gemma":[0.000817971,0.00032131275,0.0005590125,0.0004583057,0.0006396174,0.00057002524,0.00073909457,0.00048089278,0.00021576996],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000099888,0.000071906434,0.0104223015,0.000091378985,0.00005698116,0.0007979458,0.00030094205,0.7755812,0.020696882,0.18169056,0.0006654179,0.0095245335],"study_design_scores_gemma":[0.000040160863,0.000071473936,0.0026298447,0.000015510837,0.00002380104,0.00020026961,0.000061321116,0.9597439,0.0013833608,0.03397685,0.001829177,0.000024285662],"about_ca_topic_score_codex":0.0033077723,"about_ca_topic_score_gemma":0.0017428667,"teacher_disagreement_score":0.0033077723,"about_ca_system_score_codex":0.00046909074,"about_ca_system_score_gemma":0.0003271483,"threshold_uncertainty_score":0.006577015},"labels":[],"label_agreement":null},{"id":"W1978276672","doi":"10.1088/0004-637x/729/1/64","title":"POLYCYCLIC AROMATIC HYDROCARBON FAR-INFRARED SPECTROSCOPY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Coronene; Spectral line; Physics; Infrared spectroscopy; Polycyclic aromatic hydrocarbon; Spectroscopy; Infrared; Molecular physics; Molecule; Optics","score_opus":0.01385537547284629,"score_gpt":0.22957520065478798,"score_spread":0.2157198251819417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978276672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8050464,0.008658187,0.09821188,0.00023266875,0.00024148611,0.00021987688,0.018234167,0.0016013775,0.067554064],"genre_scores_gemma":[0.92884004,0.0039703017,0.042858697,0.00016032514,0.00004729937,0.000106920845,0.0076956768,0.00009758827,0.016223157],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9995964,0.00003395672,0.000008803332,0.00010044401,0.00022303933,0.00003726757],"domain_scores_gemma":[0.9998049,0.000038653765,0.000024125045,0.0000280623,0.00009199343,0.000012305709],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031546698,0.00036479815,0.00026803347,0.0013182643,0.0005418277,0.00029333646,0.00051849073,0.0003894132,0.007868922],"category_scores_gemma":[0.0003775688,0.00014215668,0.00027812057,0.001361778,0.0002089287,0.00054276484,0.0002992886,0.00041158983,0.0020570457],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003010808,0.00012745574,0.013431726,0.0006222016,0.00009428087,0.00028663216,0.00023195095,0.0052129976,0.9162242,0.0031442444,0.0034397074,0.05688346],"study_design_scores_gemma":[0.000039116003,0.00079728867,0.12695536,0.00014397984,0.0001476649,0.0012744343,0.000737815,0.02662852,0.7779281,0.0041986024,0.060966417,0.00018267758],"about_ca_topic_score_codex":0.0010928208,"about_ca_topic_score_gemma":0.0016290722,"teacher_disagreement_score":0.007868922,"about_ca_system_score_codex":0.00017329313,"about_ca_system_score_gemma":0.00012931737,"threshold_uncertainty_score":0.026324153},"labels":[],"label_agreement":null},{"id":"W1978308749","doi":"10.1086/320457","title":"MACHO 96‐LMC‐2: Lensing of a Binary Source in the Large Magellanic Cloud and Constraints on the Lensing Object","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gravitational microlensing; Physics; Astrophysics; Photometry (optics); Large Magellanic Cloud; Astronomy; Light curve; Gravitational lens; Binary number; Brightness; Stars; Galaxy; Redshift","score_opus":0.014930066158294755,"score_gpt":0.22948365744347943,"score_spread":0.21455359128518467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978308749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9907052,0.0002635262,0.0005205919,0.0004235387,0.000018268442,0.000011834631,0.0003931456,0.000037642603,0.0076261037],"genre_scores_gemma":[0.9980236,0.00005091905,0.00056802353,0.00003570133,0.000019987898,0.0000030264137,0.00038152924,0.000009929418,0.0009073455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998983,0.000009260585,0.000004942701,0.000028088054,0.000030872237,0.000028603718],"domain_scores_gemma":[0.9994992,0.000061544946,0.00014467222,0.000055687025,0.000035968205,0.00020289667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027452272,0.00022922984,0.00027921202,0.0008341872,0.0011013525,0.0010853631,0.00047018687,0.0007486456,0.0023970136],"category_scores_gemma":[0.0009895986,0.00019438322,0.00017377215,0.0010470169,0.00043584846,0.00052761217,0.0010490593,0.0005119343,0.0003492321],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017381383,0.0002539527,0.81913686,0.00020437573,0.00015670614,0.008545171,0.0014932654,0.0046068383,0.08361412,0.021475099,0.010543347,0.048232146],"study_design_scores_gemma":[0.00008775102,0.00008167664,0.96958655,0.000026358186,0.000042123076,0.0018125759,0.00078266696,0.011437504,0.004352618,0.0062933154,0.0054579456,0.000038933038],"about_ca_topic_score_codex":0.019237453,"about_ca_topic_score_gemma":0.02829446,"teacher_disagreement_score":0.019237453,"about_ca_system_score_codex":0.0010627279,"about_ca_system_score_gemma":0.0005292817,"threshold_uncertainty_score":0.038250983},"labels":[],"label_agreement":null},{"id":"W1978398939","doi":"10.1086/504793","title":"Microwave Emission from Spinning Dust in Circumstellar Disks","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Research Canada; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Circumstellar dust; Population; Cosmic dust","score_opus":0.00935311849952285,"score_gpt":0.22889084677489602,"score_spread":0.21953772827537316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978398939","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973653,0.00041894778,0.001308793,0.000017987146,0.0000036014762,0.0000035196924,0.000029408482,0.000031978394,0.0008205252],"genre_scores_gemma":[0.9990196,0.00018100362,0.00048339705,0.000011824042,0.000014586519,0.000003876153,0.00005323654,0.0000047017097,0.00022787885],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999653,0.000005010417,0.0000011774661,0.000013461232,0.00000769546,0.000007321718],"domain_scores_gemma":[0.9999001,0.000038366412,0.00002918103,0.000009862909,0.00000811519,0.000014309927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007010222,0.00016702662,0.00014447681,0.00030388465,0.00018495468,0.00032239285,0.00026398856,0.00023695495,0.0006748581],"category_scores_gemma":[0.00025452572,0.00014390869,0.00009350021,0.00022117986,0.0002598458,0.00019427539,0.00018528386,0.00013514371,0.00022814551],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039346298,0.00014538575,0.10491829,0.00015737319,0.000055465796,0.0010909091,0.00043381928,0.0021737455,0.86764985,0.00090739585,0.00035722862,0.021717133],"study_design_scores_gemma":[0.00012808891,0.00053211517,0.8335225,0.000030678195,0.00009416058,0.0022508656,0.00043999616,0.015621341,0.14122109,0.002199037,0.0039307848,0.00002930144],"about_ca_topic_score_codex":0.000223466,"about_ca_topic_score_gemma":0.0001548983,"teacher_disagreement_score":0.0006748581,"about_ca_system_score_codex":0.0001171259,"about_ca_system_score_gemma":0.000023862853,"threshold_uncertainty_score":0.0022575855},"labels":[],"label_agreement":null},{"id":"W1978473915","doi":"10.1088/0004-637x/802/2/73","title":"AVOIDING PROGENITOR BIAS: THE STRUCTURAL AND MASS EVOLUTION OF BRIGHTEST GROUP AND CLUSTER GALAXIES IN HIERARCHICAL MODELS SINCE<i>z</i>≲ 1","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Stellar mass; Galaxy; Redshift; Halo; Galaxy formation and evolution; Galaxy cluster; Cluster (spacecraft); Local Group","score_opus":0.015503510099135488,"score_gpt":0.2164026362296601,"score_spread":0.20089912613052463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978473915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977124,0.00007418427,0.001247563,0.00008825485,0.0000016790493,0.000003844827,0.0001142729,0.000021518574,0.00073634944],"genre_scores_gemma":[0.999022,0.00003179225,0.00044589376,0.000019972662,0.0000036023569,0.0000031399857,0.00022011549,0.000014037026,0.00023944635],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998388,0.000043067903,0.000005019013,0.000056041164,0.000016912583,0.00004010291],"domain_scores_gemma":[0.99867225,0.00040253834,0.00039820067,0.00014596844,0.00007949899,0.00030154464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011967015,0.00028140075,0.0003202076,0.0006110863,0.00045342487,0.0012527263,0.00077368564,0.00036399948,0.0009459047],"category_scores_gemma":[0.0031823702,0.00024062039,0.0004549701,0.00039447504,0.0006114288,0.0007938433,0.0007635247,0.00035522503,0.00020464598],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045528106,0.00009171736,0.9020893,0.00004284377,0.00017434184,0.00018610984,0.0011300439,0.072458446,0.003737412,0.009908339,0.0008454715,0.008880769],"study_design_scores_gemma":[0.000056407775,0.0001450991,0.5300704,0.000028161678,0.00014826827,0.00012099573,0.00078958407,0.45429197,0.0012013036,0.011971542,0.0011371068,0.00003916112],"about_ca_topic_score_codex":0.037532866,"about_ca_topic_score_gemma":0.03170153,"teacher_disagreement_score":0.037532866,"about_ca_system_score_codex":0.0011579919,"about_ca_system_score_gemma":0.00044768208,"threshold_uncertainty_score":0.07462883},"labels":[],"label_agreement":null},{"id":"W1978505139","doi":"10.1088/0004-637x/796/2/81","title":"NON-THERMAL GAMMA-RAY EMISSION FROM DELAYED PAIR BREAKDOWN IN A MAGNETIZED AND PHOTON-RICH OUTFLOW","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Lorentz factor; Compton scattering; Outflow; Scattering; Particle acceleration; Magnetohydrodynamics; Photon; Spectral line; Radiative transfer","score_opus":0.004175590704153459,"score_gpt":0.19732620264841083,"score_spread":0.19315061194425737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978505139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960064,0.000064773485,0.001928294,0.000061026833,0.000005739775,0.000010268513,0.00007549791,0.000047525475,0.0018005912],"genre_scores_gemma":[0.99905974,0.000022051849,0.0005150252,0.000014905909,0.0000036988426,0.000006578122,0.000050814655,0.000013140928,0.00031411764],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99991846,0.00001700408,0.0000032113396,0.00001143075,0.000013003656,0.000036910107],"domain_scores_gemma":[0.9997545,0.00008643823,0.00005312238,0.000014833713,0.000022366454,0.000068706795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024348949,0.0005281677,0.00038005604,0.00034111826,0.00050945673,0.00087703485,0.0008531892,0.00060835766,0.0009481993],"category_scores_gemma":[0.000692254,0.00022866251,0.0005956074,0.00030284864,0.0008979821,0.00047309182,0.0007942697,0.0005354237,0.000093963106],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013261694,0.00037059502,0.037896276,0.00012470316,0.00014770037,0.004525115,0.00049311324,0.88574404,0.055173732,0.009960092,0.0005161541,0.0037223182],"study_design_scores_gemma":[0.00017971275,0.00024114572,0.015496818,0.000012113703,0.000029081499,0.00027427002,0.0001706991,0.97607285,0.0053953636,0.00189263,0.00020451588,0.000030876898],"about_ca_topic_score_codex":0.0049408306,"about_ca_topic_score_gemma":0.0018590267,"teacher_disagreement_score":0.0049408306,"about_ca_system_score_codex":0.001094956,"about_ca_system_score_gemma":0.00028794407,"threshold_uncertainty_score":0.009824157},"labels":[],"label_agreement":null},{"id":"W1978518200","doi":"10.1086/374301","title":"Measuring Feedback Using the Intergalactic Medium State and Evolution Inferred from the Soft X‐Ray Background","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; ROSAT; Redshift; Galaxy; X-ray background; Spectral density; Flux (metallurgy); Astronomy; Quasar; Statistics","score_opus":0.02250620151742553,"score_gpt":0.2246562886881386,"score_spread":0.2021500871707131,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978518200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99517787,0.000063890606,0.0037942354,0.00001279872,0.000001297913,0.0000034718187,0.000110495435,0.00006686451,0.00076914247],"genre_scores_gemma":[0.9987287,0.00004123733,0.00096233643,0.000006508547,0.0000021635742,0.0000030743968,0.00012457704,0.0000039243537,0.00012746078],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998969,0.000022481878,0.0000041549397,0.000029621595,0.000026016389,0.000020829413],"domain_scores_gemma":[0.99937975,0.00022525081,0.00016680846,0.000072753435,0.00006188228,0.00009356589],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003186472,0.00043179654,0.00016227512,0.0007273063,0.00015204275,0.00057408045,0.00024520227,0.0002301073,0.00073011604],"category_scores_gemma":[0.0017188968,0.00020254518,0.00018785795,0.00039624263,0.00015524164,0.0005453117,0.00055024045,0.00022599306,0.0001467455],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032351023,0.000092547765,0.87806433,0.000046773934,0.00012251764,0.00011692498,0.00018682882,0.012039918,0.0722149,0.0015293396,0.000097933465,0.035164397],"study_design_scores_gemma":[0.000023469578,0.00018487789,0.91057533,0.0000137387815,0.00009586053,0.0001267834,0.00008561986,0.065447256,0.021179281,0.001836683,0.00040993764,0.000021023094],"about_ca_topic_score_codex":0.00315025,"about_ca_topic_score_gemma":0.0046624886,"teacher_disagreement_score":0.00315025,"about_ca_system_score_codex":0.00032492122,"about_ca_system_score_gemma":0.000139109,"threshold_uncertainty_score":0.006263852},"labels":[],"label_agreement":null},{"id":"W1978615856","doi":"10.1086/588284","title":"Variability of the High Magnetic Field X-Ray Pulsar PSR J1846-0258 Associated with the Supernova Remnant Kes 75 as Revealed by the <i>Chandra X-Ray Observatory</i>","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Research Canada; University of Manitoba","funders":"","keywords":"Physics; Pulsar; Astrophysics; Pulsar wind nebula; Magnetar; Supernova remnant; X-ray pulsar; Astronomy; Luminosity; Pulsar planet; Crab Pulsar; Observatory; Supernova; Crab Nebula; Millisecond pulsar; Binary pulsar; Galaxy","score_opus":0.009863800796861194,"score_gpt":0.24653615369165144,"score_spread":0.23667235289479024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978615856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995671,0.000040657593,0.000020308691,0.000004090087,0.0000012822421,0.0000012537939,0.00006642505,0.0000042174415,0.00029469962],"genre_scores_gemma":[0.99939287,0.000031558655,0.00008295154,0.0000069123753,0.00000436483,0.0000014707193,0.00034706385,0.0000017378595,0.00013107248],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999293,0.000005261751,0.000005627791,0.000023696959,0.000019096251,0.000017051845],"domain_scores_gemma":[0.99980134,0.000010927968,0.00010902408,0.000016375248,0.000021303831,0.00004102057],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011042328,0.00016078542,0.00017175781,0.00057555834,0.00018384363,0.00042249035,0.00017415898,0.00013415687,0.0004144028],"category_scores_gemma":[0.00031906518,0.00008758414,0.00009900968,0.00034146802,0.00022822667,0.00014683045,0.0003112039,0.00013363837,0.00018831204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023166549,0.00014188397,0.94433945,0.000031419415,0.00009953448,0.00079868175,0.00023587047,0.00037256596,0.044562224,0.00015099754,0.0003716132,0.008664178],"study_design_scores_gemma":[0.0000026755197,0.000029621531,0.99881494,0.0000011619028,0.000008952066,0.00024298632,0.00002969088,0.000093060095,0.00040105078,0.0000077246295,0.0003665076,0.0000016535371],"about_ca_topic_score_codex":0.003439766,"about_ca_topic_score_gemma":0.0051079905,"teacher_disagreement_score":0.003439766,"about_ca_system_score_codex":0.00022826192,"about_ca_system_score_gemma":0.00011476843,"threshold_uncertainty_score":0.006839454},"labels":[],"label_agreement":null},{"id":"W1978642495","doi":"10.1086/509314","title":"A Revised Model for the Formation of Disk Galaxies: Low Spin and Dark Halo Expansion","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":278,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Dark matter; Halo; Galaxy; Dark matter halo; Galaxy formation and evolution; Weak gravitational lensing; Star formation","score_opus":0.007963233793897363,"score_gpt":0.21552392009215438,"score_spread":0.20756068629825702,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978642495","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5324958,0.0015653283,0.41546372,0.004169717,0.00018617432,0.00017738264,0.002124958,0.0009152454,0.04290166],"genre_scores_gemma":[0.9597811,0.0005710341,0.02679274,0.0005093133,0.00012636022,0.00013476115,0.00051739207,0.00008602288,0.011481346],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997104,0.00007802081,0.000017355997,0.0001131205,0.000033131404,0.000047962272],"domain_scores_gemma":[0.99935037,0.00018681504,0.00013914489,0.00009064854,0.0001091663,0.00012393211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008497067,0.00068123016,0.0005210876,0.0008184957,0.00046998073,0.001832716,0.0022740297,0.0008120942,0.0035845218],"category_scores_gemma":[0.0019073825,0.00041478005,0.0007825926,0.00057855365,0.0009963285,0.0018796811,0.0008666897,0.000768732,0.0012040731],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022003941,0.000113108494,0.072917484,0.00031018857,0.00017701964,0.0012469558,0.0012610435,0.23615982,0.011997578,0.6254773,0.005506347,0.04461314],"study_design_scores_gemma":[0.00014397663,0.00016312014,0.024564201,0.00007892023,0.0000918995,0.0018927458,0.00026189745,0.6827347,0.0010943513,0.27533835,0.013524083,0.00011175323],"about_ca_topic_score_codex":0.0063553597,"about_ca_topic_score_gemma":0.0035301081,"teacher_disagreement_score":0.0063553597,"about_ca_system_score_codex":0.0012910683,"about_ca_system_score_gemma":0.0005705443,"threshold_uncertainty_score":0.012636721},"labels":[],"label_agreement":null},{"id":"W1978730042","doi":"10.1088/0004-637x/780/1/70","title":"SUPERMASSIVE BLACK HOLES AND THEIR HOST GALAXIES. II. THE CORRELATION WITH NEAR-INFRARED LUMINOSITY REVISITED","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Bulge; Supermassive black hole; Luminosity; Scaling; Quasar; Hubble's law; Black hole (networking); Spiral galaxy","score_opus":0.0051795755603352275,"score_gpt":0.18128565780488315,"score_spread":0.17610608224454793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978730042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99520606,0.0022328075,0.0010240681,0.0001766697,0.00000766484,0.0000037116322,0.00011778047,0.00002161208,0.001209475],"genre_scores_gemma":[0.99911445,0.0002635312,0.00026622345,0.00003957236,0.000035156667,0.0000023442192,0.00009674498,0.000006438686,0.00017556251],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996439,0.000106240965,0.000020952471,0.00010672831,0.00006248963,0.00005972038],"domain_scores_gemma":[0.9919099,0.0033599986,0.003240336,0.00071552483,0.00028939886,0.0004848467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009351025,0.00047468973,0.00031679068,0.0014148948,0.00022486936,0.0010918524,0.0005658277,0.00066158833,0.0018746386],"category_scores_gemma":[0.005428061,0.000260529,0.0003552613,0.0013182103,0.0012833953,0.0012837896,0.00084181933,0.0008242618,0.0005145567],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006662644,0.00001276152,0.9919675,0.000013237953,0.000035470886,0.000098008706,0.00013799014,0.00025914414,0.0014670657,0.00046941146,0.000069121284,0.0054035606],"study_design_scores_gemma":[0.000002219561,0.000047556845,0.9972466,0.000008771722,0.000015146324,0.00028442062,0.00015397357,0.0010630597,0.00023343494,0.0006968398,0.00024238022,0.000005544193],"about_ca_topic_score_codex":0.0021167407,"about_ca_topic_score_gemma":0.0022624559,"teacher_disagreement_score":0.0021167407,"about_ca_system_score_codex":0.00023337983,"about_ca_system_score_gemma":0.00013159601,"threshold_uncertainty_score":0.006271243},"labels":[],"label_agreement":null},{"id":"W1978738556","doi":"10.1088/0004-637x/786/2/134","title":"<i>HUBBLE SPACE TELESCOPE</i>AND GROUND-BASED OBSERVATIONS OF THE TYPE Iax SUPERNOVAE SN 2005hk AND SN 2008A","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"U.S. Department of Energy; Vetenskapsrådet; U.S. Naval Observatory; National Science Foundation; Case Western Reserve University; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; New Mexico State University; University of Portsmouth; Universität Basel; University of Pittsburgh; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; Princeton University; Johns Hopkins University; Ohio State University; California Institute of Technology; Space Telescope Science Institute; W. M. Keck Foundation; Drexel University; National Aeronautics and Space Administration","keywords":"Physics; Supernova; Astrophysics; Ejecta; Photometry (optics); White dwarf; Hubble space telescope; Spitzer Space Telescope; Pair-instability supernova; Astronomy; Infrared; Spectral line; Stars","score_opus":0.014411687574524582,"score_gpt":0.21831271555858422,"score_spread":0.20390102798405965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978738556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9821149,0.0005235493,0.0011714328,0.000098986384,0.000039245588,0.00006117432,0.010020236,0.00023725677,0.005733268],"genre_scores_gemma":[0.945822,0.0004405329,0.009483074,0.00035162023,0.00012834466,0.0000586438,0.039939124,0.000051728297,0.0037248973],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987555,0.0000063222456,0.000009886747,0.000035076573,0.000049903763,0.000023179246],"domain_scores_gemma":[0.9992859,0.000020473168,0.00035894898,0.000048551276,0.00006768731,0.00021851128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028716025,0.00046809507,0.000242484,0.0017211722,0.0003033899,0.00042125816,0.0003850411,0.00035705758,0.0017224236],"category_scores_gemma":[0.0002521896,0.00015961929,0.00029538572,0.0006577577,0.0001919641,0.0003802356,0.00051303336,0.00031821668,0.0005683841],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029588657,0.00022732129,0.9430419,0.00012042161,0.00023544983,0.00050359033,0.0002020596,0.00061820156,0.025841082,0.0003992258,0.007701138,0.020813616],"study_design_scores_gemma":[0.000004644451,0.000054035707,0.9960001,0.0000058085384,0.000013292364,0.00018778778,0.000021876835,0.00030777275,0.0007504877,0.000037425405,0.002612873,0.0000039326155],"about_ca_topic_score_codex":0.011427046,"about_ca_topic_score_gemma":0.04277216,"teacher_disagreement_score":0.011427046,"about_ca_system_score_codex":0.0005752468,"about_ca_system_score_gemma":0.0002701073,"threshold_uncertainty_score":0.022721052},"labels":[],"label_agreement":null},{"id":"W1978805159","doi":"10.1086/374309","title":"Magnetic Structure of a Dark Bok Globule","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Linear polarization; Astrophysics; Polarization (electrochemistry); Halo; Magnetic field; Velocity dispersion; Optics; Galaxy","score_opus":0.0052202312652230515,"score_gpt":0.21481240956848663,"score_spread":0.20959217830326357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978805159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940044,0.00014652206,0.00031673853,0.00019533618,0.000028082186,0.000009007694,0.00027558062,0.00006725942,0.0049569593],"genre_scores_gemma":[0.99632096,0.000030856452,0.0002119329,0.000054959335,0.000021793869,0.000002931286,0.0003993518,0.000021703603,0.002935512],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995315,0.0000046626446,0.0000019383965,0.000013885056,0.0000102157765,0.000016131575],"domain_scores_gemma":[0.99959534,0.00004194995,0.000039686212,0.000040238818,0.00012316872,0.00015953131],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000124984,0.00011942934,0.00025716575,0.00062127,0.000628297,0.0004883645,0.00035014687,0.00029780963,0.006835133],"category_scores_gemma":[0.00045098335,0.00009389503,0.00009408738,0.00024363158,0.00040462363,0.00025472624,0.0005817215,0.00027214683,0.0013116836],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002723517,0.00015772514,0.104489684,0.00029316064,0.00013715269,0.0034661877,0.001448684,0.0016439176,0.8515941,0.005719592,0.005272088,0.023054242],"study_design_scores_gemma":[0.0002560541,0.0012962555,0.84344906,0.000027877406,0.00013380058,0.003621975,0.001969749,0.006413948,0.1054624,0.0056553087,0.031629186,0.000084499865],"about_ca_topic_score_codex":0.0017209215,"about_ca_topic_score_gemma":0.0009864531,"teacher_disagreement_score":0.006835133,"about_ca_system_score_codex":0.00032078693,"about_ca_system_score_gemma":0.00011753773,"threshold_uncertainty_score":0.022865772},"labels":[],"label_agreement":null},{"id":"W1978832586","doi":"10.1088/0004-637x/770/1/29","title":"SPECTROSCOPIC OBSERVATIONS OF SN 2012fr: A LUMINOUS, NORMAL TYPE Ia SUPERNOVA WITH EARLY HIGH-VELOCITY FEATURES AND A LATE VELOCITY PLATEAU","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Fondo de Innovación para la Competitividad; Science and Technology Facilities Council; Jet Propulsion Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; ARC Centre of Excellence for All-Sky Astrophysics; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Ministerio de Economía, Fomento y Turismo, Chile; Chinese Academy of Agricultural Sciences; National Science Foundation","keywords":"Physics; Supernova; Astrophysics; Plateau (mathematics); Astronomy","score_opus":0.010157547627973204,"score_gpt":0.21478724836959745,"score_spread":0.20462970074162423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978832586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99690825,0.00014278047,0.00030783543,0.000019082438,0.0000095383575,0.000011983889,0.0010634755,0.00006166675,0.0014754451],"genre_scores_gemma":[0.9960312,0.00008096223,0.0009266277,0.000026237152,0.00002065278,0.0000084736375,0.0022221215,0.000015550071,0.0006681392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998982,0.00000622558,0.0000070958004,0.000027531543,0.000030143336,0.00003068198],"domain_scores_gemma":[0.9997502,0.00000945142,0.00007611959,0.00002152261,0.000049834016,0.00009285322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027787383,0.0005177833,0.0002739154,0.0011659403,0.00040521324,0.00024262046,0.0002176185,0.0003931419,0.0005983516],"category_scores_gemma":[0.00024573752,0.0001944774,0.0002843097,0.00068060076,0.00014198491,0.0001967497,0.00029407738,0.00030190797,0.00027882785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009604891,0.00035921778,0.7525753,0.00011565315,0.00017331915,0.0016076991,0.0004977882,0.000722489,0.20926155,0.00035808494,0.0028889172,0.03047947],"study_design_scores_gemma":[0.0000058674627,0.00011501401,0.99580693,0.0000029704186,0.000011638081,0.0008212347,0.00003950731,0.00033685798,0.0018771798,0.00002379098,0.0009526948,0.0000063427515],"about_ca_topic_score_codex":0.0088789845,"about_ca_topic_score_gemma":0.018916925,"teacher_disagreement_score":0.0088789845,"about_ca_system_score_codex":0.00021995549,"about_ca_system_score_gemma":0.00013361302,"threshold_uncertainty_score":0.017654598},"labels":[],"label_agreement":null},{"id":"W1978841089","doi":"10.1086/308536","title":"Properties of Dust Grains in Planetary Nebulae. I. The Ionized Region of NGC 6445","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Nebula; Astrophysics; Physics; Planetary nebula; Photoionization; Ionization; Infrared; Flux (metallurgy); Reflection nebula; Luminosity; Emission nebula; Emission spectrum; Astronomy; Spectral line; Galaxy; Stars; Chemistry; Ion","score_opus":0.016322983527280913,"score_gpt":0.20793409501711713,"score_spread":0.19161111148983623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978841089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953747,0.00012880059,0.00008383558,0.0000030955816,7.694732e-7,0.0000015070958,0.000059017766,0.000005505593,0.00018007119],"genre_scores_gemma":[0.9996358,0.000026849744,0.00006570604,0.00000447206,9.603788e-7,0.0000013268213,0.00017682071,0.0000029994,0.00008508981],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999325,0.000004104831,0.0000049262767,0.000027325368,0.000014576031,0.000016609132],"domain_scores_gemma":[0.99983597,0.00002832695,0.000058247086,0.000013213466,0.000021600974,0.000042593514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000084549894,0.0001827363,0.00017973984,0.0006900454,0.00024220004,0.00045171974,0.00016997334,0.00019293076,0.00046999104],"category_scores_gemma":[0.0002522103,0.00015148589,0.00016830896,0.00026892836,0.00023222451,0.00018382454,0.00022363012,0.00010635582,0.000099625846],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030567579,0.0000573866,0.7094009,0.00004439079,0.00013330116,0.0005544919,0.00042724237,0.0014205358,0.28205675,0.00015029275,0.00012989165,0.0053191516],"study_design_scores_gemma":[0.000006901274,0.000056419005,0.99131364,0.0000022648082,0.000018474053,0.00026338542,0.00011903182,0.0013213317,0.0064712227,0.00006600014,0.00035728217,0.0000041195635],"about_ca_topic_score_codex":0.005686274,"about_ca_topic_score_gemma":0.0029486625,"teacher_disagreement_score":0.005686274,"about_ca_system_score_codex":0.00022239324,"about_ca_system_score_gemma":0.000041635238,"threshold_uncertainty_score":0.011306345},"labels":[],"label_agreement":null},{"id":"W1978849153","doi":"10.1088/0004-637x/695/1/310","title":"PERIODIC RADIO AND Hα EMISSION FROM THE L DWARF BINARY 2MASSW J0746425+200032: EXPLORING THE MAGNETIC FIELD TOPOLOGY AND RADIUS OF AN L DWARF","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Magnetic field; RADIUS; Rotation period; Starspot; Field (mathematics); Light curve; Topology (electrical circuits); Stars; Quantum mechanics","score_opus":0.014453308996990174,"score_gpt":0.22551349910508903,"score_spread":0.21106019010809884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978849153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989291,0.00013100778,0.00008254917,0.000023600827,0.0000026386804,0.0000034159827,0.00018129402,0.000018475594,0.00062789524],"genre_scores_gemma":[0.9989171,0.00007443161,0.00027949535,0.000027378337,0.000016062493,0.0000046646505,0.0004491186,0.000006196914,0.00022556519],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995506,0.0000042832517,0.000002071834,0.000014771096,0.000011847333,0.000012046233],"domain_scores_gemma":[0.9998529,0.000009119747,0.00005229746,0.000011925263,0.000013974418,0.000059771042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001222873,0.00024345744,0.000269013,0.0006071919,0.00031855877,0.00035884164,0.00023470643,0.00041902132,0.00074049894],"category_scores_gemma":[0.00017796051,0.00016135152,0.00011832311,0.00037319993,0.00019222237,0.00020910766,0.00032690447,0.0001915476,0.0003865344],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000784611,0.00020913305,0.4042089,0.00018580485,0.000099983205,0.002685497,0.0007845059,0.0008476216,0.5703521,0.00024087877,0.0011856129,0.018415324],"study_design_scores_gemma":[0.000030892472,0.00018384996,0.99102014,0.0000144109445,0.000020920781,0.0008624105,0.0001453153,0.0012558822,0.0049909162,0.00007606083,0.0013882999,0.000010930842],"about_ca_topic_score_codex":0.0015557967,"about_ca_topic_score_gemma":0.003937471,"teacher_disagreement_score":0.0015557967,"about_ca_system_score_codex":0.00020185653,"about_ca_system_score_gemma":0.000118254306,"threshold_uncertainty_score":0.003093481},"labels":[],"label_agreement":null},{"id":"W1978929779","doi":"10.1086/466522","title":"Simultaneous Ultraviolet and X‐Ray Observations of Seyfert Galaxy NGC 4151. I. Physical Conditions in the X‐Ray Absorbers","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Galaxy; Space Telescope Imaging Spectrograph; Ionization; Spectral line; Absorption (acoustics); Ultraviolet; Astronomy; Emission spectrum; Flux (metallurgy); Absorption spectroscopy; Spectrograph; Hubble space telescope; Optics; Ion; Chemistry","score_opus":0.013874441383738266,"score_gpt":0.24766422366152205,"score_spread":0.23378978227778377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1978929779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99885833,0.00011247806,0.000064872336,0.000009452854,0.0000013209809,0.0000040017167,0.00027242195,0.0000102807535,0.00066677283],"genre_scores_gemma":[0.9984194,0.0000891869,0.00036923322,0.000011575376,0.0000060565126,0.0000063813777,0.0007020936,0.000003977621,0.0003920694],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998698,0.000010290556,0.000008278494,0.0000451363,0.000030907886,0.000035609963],"domain_scores_gemma":[0.99971884,0.000029105904,0.00009810819,0.00003370572,0.000035866415,0.00008436574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018022807,0.00024468452,0.0001872451,0.0011995672,0.00061781803,0.00043509103,0.00023660458,0.00024612652,0.0010582514],"category_scores_gemma":[0.00028673076,0.00021589795,0.00017170886,0.00072712026,0.00019676037,0.00039574565,0.0005434811,0.00023983612,0.00019326014],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001136435,0.00023899405,0.7667452,0.00012676584,0.00015018956,0.001372758,0.0017596162,0.0010627917,0.20743932,0.000443593,0.00060193276,0.018922428],"study_design_scores_gemma":[0.000007646012,0.00006393069,0.99629337,0.0000042390634,0.000018585048,0.00030899787,0.00011749551,0.0001543688,0.0024403087,0.000030736126,0.000556171,0.0000041269686],"about_ca_topic_score_codex":0.0043787137,"about_ca_topic_score_gemma":0.015246639,"teacher_disagreement_score":0.0043787137,"about_ca_system_score_codex":0.00036973605,"about_ca_system_score_gemma":0.00013308114,"threshold_uncertainty_score":0.00870645},"labels":[],"label_agreement":null},{"id":"W1979176742","doi":"10.1088/0004-637x/743/1/44","title":"THE CIRCUMSTELLAR ENVIRONMENT OF R CORONAE BOREALIS: WHITE DWARF MERGER OR FINAL-HELIUM-SHELL FLASH?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; White dwarf; Astronomy; Nebula; Planetary nebula; Shell (structure); Helium; Line-of-sight; Stars","score_opus":0.025159047280207212,"score_gpt":0.21486850366423263,"score_spread":0.18970945638402542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979176742","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98960704,0.005694463,0.00025342318,0.0004766485,0.000046516692,0.000012803697,0.00015718471,0.000041604184,0.0037103214],"genre_scores_gemma":[0.99903166,0.00040986895,0.00008198294,0.0001096235,0.000049485272,0.0000010747418,0.00012806428,0.0000024927822,0.00018570725],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985075,0.00001035089,0.0000105193285,0.000049844686,0.000026958802,0.0000516382],"domain_scores_gemma":[0.9997193,0.000016291648,0.00016015739,0.000015658428,0.00001739778,0.00007113871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024533182,0.00030206257,0.00028626886,0.00041292407,0.0005524537,0.00072091946,0.0003572086,0.00072275475,0.0013573884],"category_scores_gemma":[0.00048377877,0.0001052291,0.00022984942,0.00026949664,0.0007197476,0.00056896865,0.0004522469,0.00029101025,0.00027794112],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069245225,0.00011107186,0.91075546,0.0002454295,0.00015207865,0.016262233,0.000916877,0.000058782985,0.046259776,0.00066956034,0.0013180955,0.02255819],"study_design_scores_gemma":[0.000014271748,0.00016313708,0.97272044,0.000024764668,0.000045116005,0.020924693,0.00073801976,0.00007059582,0.0011405597,0.00028477373,0.0038633458,0.000010249844],"about_ca_topic_score_codex":0.002316823,"about_ca_topic_score_gemma":0.0038160346,"teacher_disagreement_score":0.002316823,"about_ca_system_score_codex":0.0003582771,"about_ca_system_score_gemma":0.00013882226,"threshold_uncertainty_score":0.004606724},"labels":[],"label_agreement":null},{"id":"W1979235198","doi":"10.1086/496913","title":"Virial Masses and the Baryon Fraction in Galaxies","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Victoria; University of Toronto","funders":"","keywords":"Virial mass; Galaxy; Virial theorem; Baryon; Stellar mass; Redshift; Luminosity function; Luminosity; Galaxy cluster","score_opus":0.005407844025422352,"score_gpt":0.2099303163247991,"score_spread":0.20452247229937676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979235198","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99883336,0.00012360803,0.00050931354,0.000009019054,7.584394e-7,0.0000013150427,0.00011004363,0.000021374597,0.00039131733],"genre_scores_gemma":[0.9993814,0.000023456561,0.00021289087,0.000003105299,0.0000017823253,0.0000010147958,0.0002459194,0.0000034248837,0.00012704331],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976784,0.000034573062,0.000018828374,0.00007699267,0.000048103557,0.00005366882],"domain_scores_gemma":[0.99798065,0.000513791,0.0008134838,0.0002655602,0.00019388522,0.00023264141],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005600122,0.00031705538,0.0002413713,0.0015615886,0.0002767003,0.0009480191,0.00041110397,0.00021315992,0.0010407036],"category_scores_gemma":[0.0033232807,0.00016032768,0.00021780924,0.00075965683,0.00057082553,0.0005169279,0.00065587607,0.00021871326,0.00023768694],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024174397,0.000047444402,0.9377891,0.00004033099,0.00012710626,0.000054524127,0.00039376444,0.0027222433,0.04450145,0.0017335906,0.000078749836,0.012270024],"study_design_scores_gemma":[0.0000060000634,0.00006737737,0.98733634,0.000007750751,0.000028726652,0.00012784477,0.00006002951,0.0034665354,0.0077060317,0.00080606743,0.00037195816,0.000015316937],"about_ca_topic_score_codex":0.002634261,"about_ca_topic_score_gemma":0.0027959836,"teacher_disagreement_score":0.002634261,"about_ca_system_score_codex":0.0005986976,"about_ca_system_score_gemma":0.000111070316,"threshold_uncertainty_score":0.005237937},"labels":[],"label_agreement":null},{"id":"W1979356384","doi":"10.1088/0004-637x/766/1/46","title":"SEARCH FOR HIGH PROPER MOTION OBJECTS IN THE CFHTLS DEEP FIELDS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Proper motion; Astrophysics; White dwarf; Galaxy; Halo; Quasar; Astronomy; Telescope; Thick disk; Spectral energy distribution; Thin disk; Stars","score_opus":0.010071485059136884,"score_gpt":0.21988194423333393,"score_spread":0.20981045917419705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979356384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968008,0.0001066736,0.00023889595,0.00004041139,0.0000030922715,0.000010865081,0.0019963447,0.000028745084,0.0007742067],"genre_scores_gemma":[0.9906673,0.00006327065,0.0008917713,0.00006668426,0.000016198866,0.000016048516,0.007492857,0.000009361195,0.000776456],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996107,0.000026730753,0.000013358718,0.00009672281,0.00008806217,0.00016439818],"domain_scores_gemma":[0.99761814,0.00023580635,0.00065730826,0.00021776662,0.00025781308,0.0010131468],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007588273,0.00037896508,0.0003386837,0.003935258,0.00071374263,0.0006208387,0.00039720174,0.00028133823,0.0016456274],"category_scores_gemma":[0.0011208882,0.00019929235,0.00022929147,0.0020440922,0.00032417924,0.00037298384,0.0009923569,0.00026411167,0.0003054753],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000070569906,0.00004757331,0.98157513,0.000013922277,0.00004008769,0.00019580706,0.00034422035,0.00018508114,0.006940808,0.00018737717,0.0013065772,0.009092897],"study_design_scores_gemma":[0.0000051343495,0.000020484858,0.9981007,0.000002936315,0.0000074562636,0.000069647685,0.00009203829,0.00020623296,0.0003678543,0.000037209462,0.0010857059,0.0000046101895],"about_ca_topic_score_codex":0.046397645,"about_ca_topic_score_gemma":0.110310234,"teacher_disagreement_score":0.046397645,"about_ca_system_score_codex":0.0009823196,"about_ca_system_score_gemma":0.0006641871,"threshold_uncertainty_score":0.092255175},"labels":[],"label_agreement":null},{"id":"W1979518349","doi":"10.1086/595870","title":"Direct Imaging and Spectroscopy of a Planetary-Mass Candidate Companion to a Young Solar Analog","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":232,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetary mass; Planet; Physics; Solar mass; Astrophysics; Astronomy; Spectroscopy; Solar System; Brown dwarf; Surface gravity; Planetary science; Planetary system; Spectral line; Stars","score_opus":0.007459282936516453,"score_gpt":0.21563671507282117,"score_spread":0.2081774321363047,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979518349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979785,0.00009583881,0.00023364568,0.00004164964,0.000002592257,0.0000032005794,0.00006679872,0.00002180054,0.0015560448],"genre_scores_gemma":[0.99797064,0.000050036782,0.0010083409,0.00003358862,0.000010626404,0.000003933334,0.0002694009,0.0000051709158,0.0006483537],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999535,0.000003495259,0.0000017209742,0.000017726505,0.000012531051,0.000011089113],"domain_scores_gemma":[0.9999058,0.000010244727,0.000026000425,0.000012690739,0.000012274319,0.00003293272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001265822,0.0001308243,0.00012439095,0.00045573147,0.00033805452,0.00024486866,0.00023984528,0.0004623816,0.001002489],"category_scores_gemma":[0.00018357125,0.00013502469,0.00009039548,0.00019242446,0.00013837926,0.000222754,0.00035636115,0.00019675739,0.00029752895],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030198426,0.0001719516,0.18869907,0.000074615156,0.000031735613,0.0035850508,0.00064702256,0.0004550443,0.7905081,0.00072912045,0.0009875739,0.013808704],"study_design_scores_gemma":[0.000025359752,0.00037735555,0.9497669,0.00001365931,0.00004592798,0.008228628,0.00044288655,0.0030603574,0.032051496,0.00035874016,0.0056157573,0.000012952259],"about_ca_topic_score_codex":0.00046898788,"about_ca_topic_score_gemma":0.001067164,"teacher_disagreement_score":0.001002489,"about_ca_system_score_codex":0.00014459685,"about_ca_system_score_gemma":0.000055830857,"threshold_uncertainty_score":0.0033536553},"labels":[],"label_agreement":null},{"id":"W1979656146","doi":"10.1088/0004-637x/736/2/98","title":"INTERNAL γγ OPACITY IN ACTIVE GALACTIC NUCLEI AND THE CONSEQUENCES FOR THE TeV OBSERVATIONS OF M87 AND Cen A","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Active galactic nucleus; Supermassive black hole; Centaurus A; Black hole (networking); Opacity; Luminosity; Intermediate-mass black hole; Photon; Stars","score_opus":0.0326166006158129,"score_gpt":0.23732398754053274,"score_spread":0.20470738692471985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979656146","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99797326,0.00020517659,0.00077845546,0.000022132966,0.0000022247953,0.0000023584732,0.00006717284,0.00002116031,0.0009280197],"genre_scores_gemma":[0.99965894,0.000055062643,0.00011479697,0.000006516573,0.000002914892,0.000001605145,0.00008186935,0.0000062658396,0.00007206812],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998184,0.000035068682,0.00001436291,0.00003703751,0.000045459652,0.000049717506],"domain_scores_gemma":[0.9982608,0.000818169,0.00048366943,0.00017792764,0.00010904207,0.00015051164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005724647,0.0003840877,0.00034810262,0.00076452544,0.00029703212,0.0013662246,0.0005932497,0.00041346665,0.0006770694],"category_scores_gemma":[0.0025889075,0.00022763034,0.00055333314,0.0005139038,0.00071329315,0.00032938845,0.00058679277,0.0003384602,0.00012528828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022092063,0.000037356094,0.92866564,0.00005371403,0.00012759691,0.001072366,0.00020451957,0.041607745,0.018622102,0.003994003,0.00016641078,0.0052276584],"study_design_scores_gemma":[0.00002054698,0.00007071055,0.88734406,0.000039387065,0.0001421672,0.00047444738,0.00020712269,0.10152213,0.00798648,0.001664904,0.0005087942,0.00001934336],"about_ca_topic_score_codex":0.0045875837,"about_ca_topic_score_gemma":0.002940856,"teacher_disagreement_score":0.0045875837,"about_ca_system_score_codex":0.00062866596,"about_ca_system_score_gemma":0.00013751976,"threshold_uncertainty_score":0.009121776},"labels":[],"label_agreement":null},{"id":"W1979682204","doi":"10.1086/590182","title":"Clustering of Supernova Ia Host Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"","score_opus":0.015210427543830658,"score_gpt":0.23409112074740107,"score_spread":0.21888069320357043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979682204","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974082,0.00019521429,0.00022588937,0.00005420926,0.000013727412,0.0000045315674,0.00046678365,0.000040296007,0.0015911433],"genre_scores_gemma":[0.9977533,0.000054837943,0.000113990995,0.00001582111,0.000019255125,0.0000018335182,0.0006092379,0.000012938368,0.0014187349],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962425,0.00005498202,0.0000298005,0.000119243276,0.0000671771,0.00010450824],"domain_scores_gemma":[0.9955017,0.0007395227,0.0011028928,0.00069589796,0.0009767826,0.0009830837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039035783,0.00017261453,0.00029867745,0.0021732822,0.0004410719,0.0012097274,0.00047794246,0.00031127187,0.008276133],"category_scores_gemma":[0.0023640944,0.00021531495,0.00028846753,0.0011282015,0.0003794873,0.00031209885,0.0006045659,0.0002551672,0.0013216485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018574363,0.000024448125,0.9809085,0.000019719344,0.00016886846,0.00008073542,0.00022080417,0.00063538953,0.009654554,0.00046178995,0.0014565553,0.0061829197],"study_design_scores_gemma":[0.0000045940055,0.000026475154,0.99843913,0.0000026087882,0.000019270767,0.00010171473,0.00016349967,0.00039943823,0.00027911025,0.00013032932,0.00042995514,0.000003786816],"about_ca_topic_score_codex":0.004054473,"about_ca_topic_score_gemma":0.0054149297,"teacher_disagreement_score":0.008276133,"about_ca_system_score_codex":0.0003472824,"about_ca_system_score_gemma":0.0002799701,"threshold_uncertainty_score":0.027686417},"labels":[],"label_agreement":null},{"id":"W1979697366","doi":"10.1088/0004-637x/710/2/1343","title":"FRAGMENTATION AND EVOLUTION OF MOLECULAR CLOUDS. II. THE EFFECT OF DUST HEATING","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Stars; Radiative transfer; Isothermal process; Star formation; Fragmentation (computing); Luminosity; Radiant heating; Distribution function; Stellar evolution","score_opus":0.003185396067256061,"score_gpt":0.225565176001135,"score_spread":0.22237977993387892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979697366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99597895,0.0001715887,0.0016926915,0.00010581713,0.000008132691,0.000025696749,0.0001587613,0.000065676104,0.0017927353],"genre_scores_gemma":[0.9984842,0.00005950984,0.001007728,0.000026309546,0.000004739091,0.000010759363,0.000118893804,0.000022521395,0.00026536043],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99977773,0.00006184106,0.000011499617,0.000034336757,0.000037564667,0.000077116514],"domain_scores_gemma":[0.9989537,0.00039006685,0.00021531453,0.00013262765,0.00010784794,0.00020035786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005763494,0.00058927224,0.0004916977,0.0005663076,0.0008209661,0.0007949432,0.0010158994,0.0009781474,0.0012575279],"category_scores_gemma":[0.0027048306,0.000388454,0.0007295405,0.0005349834,0.00081554236,0.0008728619,0.00074486784,0.0005405853,0.00022030095],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017236764,0.00013576311,0.04641341,0.00004769271,0.00009051522,0.00032219288,0.0001814419,0.9390094,0.007639342,0.0023753254,0.000272065,0.0033404862],"study_design_scores_gemma":[0.000113404756,0.00014371212,0.023332804,0.000013066065,0.000028408162,0.000119062934,0.000099389305,0.97040594,0.0031693152,0.002153198,0.00040114898,0.000020461594],"about_ca_topic_score_codex":0.01655268,"about_ca_topic_score_gemma":0.007651868,"teacher_disagreement_score":0.01655268,"about_ca_system_score_codex":0.0021420075,"about_ca_system_score_gemma":0.0005112862,"threshold_uncertainty_score":0.03291267},"labels":[],"label_agreement":null},{"id":"W1979729838","doi":"10.1088/0004-637x/778/2/179","title":"AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD-SOUTH: THE AGN FRACTION AND X-RAY PROPERTIES OF SUBMILLIMETER GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council; University of Science and Technology of China; National Natural Science Foundation of China; Leverhulme Trust; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Chandra Deep Field South; Redshift; Luminosity; Luminosity function; Astronomy; Submillimeter Array; Star formation; Luminous infrared galaxy; Flux (metallurgy); Hubble Deep Field","score_opus":0.014981244759461217,"score_gpt":0.21578761951945635,"score_spread":0.20080637475999513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979729838","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982691,0.00012627126,0.0002515931,0.00002420499,0.0000036591289,0.000004615165,0.0006306607,0.000029911189,0.0006598875],"genre_scores_gemma":[0.99784946,0.00006783786,0.00071869546,0.000034782803,0.000014942188,0.000006883065,0.0010328104,0.000007049848,0.00026751444],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998288,0.000024894089,0.000010334675,0.0000623304,0.00003216214,0.0000413454],"domain_scores_gemma":[0.99925095,0.00009932575,0.00027831105,0.00011954722,0.00008832496,0.00016357364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037610758,0.00020458784,0.00018640004,0.0014441713,0.00026723504,0.0005651922,0.00028550925,0.00016386124,0.001154169],"category_scores_gemma":[0.00065759727,0.00012929813,0.00021953497,0.0009493388,0.00020714094,0.00043231633,0.00052243844,0.00022269857,0.00039079826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059090202,0.00002356115,0.9818496,0.000013315465,0.000035941164,0.000060828577,0.00015053623,0.000076121185,0.007668589,0.00011937517,0.000490337,0.0094526885],"study_design_scores_gemma":[0.000002384477,0.000010094551,0.99872345,0.0000023935424,0.000008211337,0.00008271987,0.000042532814,0.00015447756,0.00042521989,0.000021566548,0.00052516785,0.0000017521436],"about_ca_topic_score_codex":0.006770049,"about_ca_topic_score_gemma":0.011465792,"teacher_disagreement_score":0.006770049,"about_ca_system_score_codex":0.0001999433,"about_ca_system_score_gemma":0.00018715051,"threshold_uncertainty_score":0.013461292},"labels":[],"label_agreement":null},{"id":"W1979765628","doi":"10.1086/339858","title":"Nonlinear Couplings between<i>r</i>‐Modes of Rotating Neutron Stars","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Polytropic process; Instability; Nonlinear system; Classical mechanics; Polytrope; Mode coupling; Neutron star; Dimensionless quantity; Linear stability; Normal mode; Quantum electrodynamics; Quantum mechanics","score_opus":0.0214131319901107,"score_gpt":0.3053594538873581,"score_spread":0.2839463218972474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979765628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897898,0.00006701193,0.007865805,0.000035522055,0.0000034660372,0.0000051880306,0.000008726932,0.000024154868,0.0022003162],"genre_scores_gemma":[0.99846137,0.000047734848,0.0010042301,0.0000056661265,0.000002591659,0.0000032490727,0.00001126296,0.000008322648,0.00045550865],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999342,0.000017853337,0.0000040660984,0.000011734504,0.000020153993,0.000011977501],"domain_scores_gemma":[0.99969745,0.00008276857,0.00013420131,0.000019244517,0.000026125632,0.000040240007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024503167,0.00030497712,0.00015299108,0.0005003416,0.00027621663,0.00043079132,0.00032217902,0.0002500146,0.000962827],"category_scores_gemma":[0.0010984496,0.00029716638,0.0001617508,0.00016824703,0.0005388542,0.00048557448,0.0006334746,0.000364645,0.00016638049],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005454557,0.0001426572,0.05769092,0.00021073963,0.000107024294,0.0012024932,0.0012276962,0.46890047,0.28242734,0.16232441,0.0007514844,0.024469234],"study_design_scores_gemma":[0.0000392587,0.00009763707,0.020818086,0.00002105166,0.000031439773,0.00030171635,0.00021669603,0.9287632,0.016935894,0.032006044,0.00072256057,0.000046358302],"about_ca_topic_score_codex":0.0013393761,"about_ca_topic_score_gemma":0.0008501869,"teacher_disagreement_score":0.0013393761,"about_ca_system_score_codex":0.00036366982,"about_ca_system_score_gemma":0.00014451747,"threshold_uncertainty_score":0.0032209754},"labels":[],"label_agreement":null},{"id":"W1979773910","doi":"10.1086/523697","title":"Cooling, Gravity, and Geometry: Flow‐driven Massive Core Formation","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":196,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Nautical Research Society","funders":"","keywords":"Physics; Core (optical fiber); Mass distribution; Gravitation; Gravity current; Thermal; Gravitational collapse; Flow (mathematics); Mechanics; Molecular cloud; Classical mechanics; Astrophysics; Meteorology; Galaxy","score_opus":0.01804509884158838,"score_gpt":0.24274279087558628,"score_spread":0.2246976920339979,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979773910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927289,0.000077874036,0.0041182167,0.00016173928,0.00001554212,0.000017627524,0.000058394693,0.000040746087,0.002780915],"genre_scores_gemma":[0.9987317,0.000029680195,0.00066975446,0.000020232936,0.000009846255,0.000008649134,0.00002464903,0.00001386167,0.0004917185],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991465,0.000024752968,0.0000014381118,0.0000110847495,0.000007165341,0.00004089459],"domain_scores_gemma":[0.99949646,0.00017185905,0.0001307259,0.00002822566,0.000036955942,0.00013580734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003558577,0.000401274,0.0004341818,0.00032773113,0.0005245691,0.00072011235,0.001005662,0.0007237852,0.0016221004],"category_scores_gemma":[0.0020969412,0.00035740837,0.0006235737,0.0002382435,0.0015855129,0.00091611774,0.00072780484,0.0004999871,0.00011867317],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015343759,0.0001063769,0.01805898,0.000023819388,0.000045517387,0.0004112022,0.000091098475,0.956732,0.004822743,0.017271552,0.00048811262,0.0017952328],"study_design_scores_gemma":[0.000070000315,0.000046561472,0.004341195,0.0000024727892,0.000009734522,0.000039160637,0.000020787033,0.9928703,0.0003779792,0.0020840596,0.00012869491,0.000009111465],"about_ca_topic_score_codex":0.023767965,"about_ca_topic_score_gemma":0.008425457,"teacher_disagreement_score":0.023767965,"about_ca_system_score_codex":0.0014910813,"about_ca_system_score_gemma":0.0007453436,"threshold_uncertainty_score":0.04725927},"labels":[],"label_agreement":null},{"id":"W1979788119","doi":"10.1088/0004-637x/691/1/261","title":"<i>SUZAKU</i>OBSERVATIONS OF LOCAL ULTRALUMINOUS INFRARED GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Spectral line; Quasar; Luminosity; Luminous infrared galaxy; Infrared; Absorption (acoustics); Astronomy; Optics","score_opus":0.014750185106388576,"score_gpt":0.22597827365397577,"score_spread":0.2112280885475872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979788119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9853338,0.00043044332,0.0010851367,0.000059985225,0.000014557697,0.000027021657,0.009921104,0.00027085244,0.0028570925],"genre_scores_gemma":[0.9549317,0.0003038774,0.004403038,0.00013411068,0.00007381897,0.00005390549,0.038489264,0.0000696318,0.0015406567],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998217,0.00001693741,0.00001612364,0.000040963503,0.000044339828,0.000059954713],"domain_scores_gemma":[0.999283,0.000050913724,0.0003041324,0.00011383102,0.00010178817,0.00014643456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026383682,0.00041798025,0.00028351526,0.002467051,0.0004331353,0.00057220424,0.00035227352,0.00020981947,0.0018131722],"category_scores_gemma":[0.0003497554,0.00013902587,0.00040001518,0.0018302683,0.00022358386,0.00023720789,0.0006385892,0.00018790884,0.0009664195],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019645483,0.000121213896,0.9378413,0.00013978417,0.00021559045,0.00055235747,0.0005138249,0.00096371176,0.033869945,0.00039708777,0.006889716,0.018298967],"study_design_scores_gemma":[0.0000033799,0.000029884928,0.9932209,0.0000038526923,0.00003133168,0.00013311335,0.00007051027,0.00029521904,0.002127861,0.00002801994,0.004049493,0.0000063361035],"about_ca_topic_score_codex":0.008662311,"about_ca_topic_score_gemma":0.016336596,"teacher_disagreement_score":0.008662311,"about_ca_system_score_codex":0.00026261163,"about_ca_system_score_gemma":0.00017152722,"threshold_uncertainty_score":0.017223775},"labels":[],"label_agreement":null},{"id":"W1979896296","doi":"10.1086/523794","title":"Limits on Mass and Radius for the Millisecond‐Period X‐Ray Pulsar SAX J1808.4−3658","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Alberta; University of Calgary","funders":"","keywords":"Neutron star; Physics; Millisecond pulsar; RADIUS; Astrophysics; Rotation period; Light curve; Millisecond; Astronomy; Stars","score_opus":0.021321310608247095,"score_gpt":0.30017581510169916,"score_spread":0.27885450449345206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979896296","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942068,0.00057218637,0.0031023289,0.000091801354,0.0000047605095,0.0000049363803,0.0003166369,0.00006627968,0.0016343322],"genre_scores_gemma":[0.9972562,0.00019668856,0.0014242014,0.000020294076,0.000015169454,0.000008788428,0.0009516273,0.000014459065,0.000112498536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997464,0.000051532166,0.000028103024,0.00006714872,0.00006173759,0.00004508096],"domain_scores_gemma":[0.99701893,0.0019007815,0.0005249945,0.00031211303,0.00011920399,0.00012401285],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009138719,0.00043230437,0.0004962315,0.0007879561,0.0003695292,0.0008600598,0.0005652245,0.0004536759,0.0008570497],"category_scores_gemma":[0.0034445256,0.0003177244,0.0004823667,0.00046435313,0.0004319633,0.00057745347,0.00090849184,0.00032208808,0.00020955596],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0027819008,0.00013498522,0.72437096,0.00041712023,0.00044476087,0.0014640174,0.0009876691,0.056333575,0.14295016,0.020227386,0.0016142719,0.048273213],"study_design_scores_gemma":[0.00035669244,0.00042151066,0.78166866,0.0001598451,0.00032925387,0.002131754,0.00046242666,0.15036179,0.03204877,0.021246323,0.010697631,0.00011534983],"about_ca_topic_score_codex":0.0011575304,"about_ca_topic_score_gemma":0.0010920053,"teacher_disagreement_score":0.0011575304,"about_ca_system_score_codex":0.00030224782,"about_ca_system_score_gemma":0.00014817886,"threshold_uncertainty_score":0.004833102},"labels":[],"label_agreement":null},{"id":"W1979908178","doi":"10.1088/0004-637x/742/2/90","title":"ELECTROMAGNETIC EXTRACTION OF ENERGY FROM BLACK-HOLE–NEUTRON-STAR BINARIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Neutron star; Gravitational wave; Poynting vector; LIGO; X-ray burster; Black hole (networking); Stellar black hole; Exotic star; X-ray binary","score_opus":0.013805441975935466,"score_gpt":0.27496419925320403,"score_spread":0.26115875727726856,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1979908178","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93032855,0.007060398,0.042825155,0.00024407645,0.00024273475,0.000049371873,0.0008053852,0.00040950184,0.018034685],"genre_scores_gemma":[0.9894973,0.0014241632,0.0055978587,0.00012690015,0.00011003333,0.000017173314,0.0007209923,0.00009660502,0.0024089504],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99992263,0.0000086898835,0.0000023324153,0.000021903044,0.000026795278,0.000017565953],"domain_scores_gemma":[0.99989545,0.000023911682,0.0000414993,0.000015228409,0.000008235034,0.0000156895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002657345,0.00027155122,0.00022669682,0.000642778,0.0003702242,0.00068088295,0.00032087683,0.00029081528,0.0019052887],"category_scores_gemma":[0.00044449794,0.00015041945,0.00008763594,0.0007867837,0.00032570277,0.0005644484,0.0009215579,0.0003231221,0.00052635965],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017046909,0.00024927326,0.06511097,0.00046334477,0.00013652536,0.0014004336,0.00041998347,0.0039215367,0.7989327,0.022164946,0.0030396648,0.10245587],"study_design_scores_gemma":[0.00015991388,0.00051863363,0.20784354,0.00010962068,0.00013652719,0.0023160987,0.00024016002,0.05870164,0.6803325,0.023104887,0.026443195,0.00009328067],"about_ca_topic_score_codex":0.00016436246,"about_ca_topic_score_gemma":0.00025903646,"teacher_disagreement_score":0.0019052887,"about_ca_system_score_codex":0.00021792142,"about_ca_system_score_gemma":0.00008490693,"threshold_uncertainty_score":0.0063738227},"labels":[],"label_agreement":null},{"id":"W1980071787","doi":"10.1088/0004-637x/780/2/189","title":"ERRATUM: “ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. III. MEASUREMENT BIASES AND COSMOLOGICAL EVOLUTION OF GAS AND STELLAR MASS FRACTIONS” (2013, ApJ, 777, 123)","year":2013,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Deutsche Forschungsgemeinschaft; University of Cambridge","keywords":"Physics; Astrophysics; Cluster (spacecraft); Galaxy groups and clusters; Astronomy; Galaxy cluster; Galaxy","score_opus":0.026951591594471642,"score_gpt":0.2277395927615867,"score_spread":0.20078800116711507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980071787","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00050234457,0.0020031398,0.00046009908,0.049660776,0.9260183,0.000039223574,0.0055602165,0.0004910703,0.015264758],"genre_scores_gemma":[0.012558728,0.01121435,0.0048534735,0.112110496,0.18497829,0.00024273305,0.02129773,0.003083957,0.6496602],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9976527,0.00020461151,0.00047174894,0.00031772646,0.0011649034,0.00018827114],"domain_scores_gemma":[0.9877994,0.0019155882,0.00068774,0.00069468183,0.008358172,0.0005445397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020303705,0.0020218955,0.0016259807,0.0038415403,0.0041412083,0.003882283,0.0026672208,0.0032343839,0.049209908],"category_scores_gemma":[0.021744534,0.00092642003,0.0011818644,0.0038979482,0.0015182529,0.0027358346,0.0020170538,0.0070125526,0.04035519],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000016260921,0.0000043084433,0.000060942555,0.00002857538,0.0000032386924,0.000045772198,0.00001067111,0.000021219568,0.00002117972,0.00030679474,0.99739707,0.00208387],"study_design_scores_gemma":[0.00002744946,0.000016415554,0.0026781573,0.00026411848,0.000027853343,0.00018621911,0.00012325092,0.00013865551,0.00035719524,0.0011792734,0.9949586,0.000042884956],"about_ca_topic_score_codex":0.06366709,"about_ca_topic_score_gemma":0.089320965,"teacher_disagreement_score":0.06366709,"about_ca_system_score_codex":0.0043824012,"about_ca_system_score_gemma":0.0059527988,"threshold_uncertainty_score":0.16462356},"labels":[],"label_agreement":null},{"id":"W1980080717","doi":"10.1086/429403","title":"Modeling Star Formation in Dwarf Spheroidal Galaxies: A Case for Extended Dark Matter Halos","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Dwarf galaxy; Dwarf spheroidal galaxy; Dark matter; Dwarf galaxy problem; Dark matter halo; Galaxy; Globular cluster; Virial mass; Stars; Dark galaxy","score_opus":0.011181402187585083,"score_gpt":0.22935260733112975,"score_spread":0.21817120514354466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980080717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9211527,0.00093267,0.07036365,0.000780577,0.00004292742,0.000063888445,0.00048373372,0.00029431487,0.0058854525],"genre_scores_gemma":[0.99140453,0.00041923393,0.0058675613,0.00006027134,0.000038121823,0.00003442716,0.00011117633,0.000038567367,0.0020260864],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998266,0.000061576546,0.000009554008,0.00003442434,0.00002040528,0.000047507492],"domain_scores_gemma":[0.9993032,0.00021394392,0.00012152827,0.00008377182,0.000072942865,0.00020458289],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076071336,0.00050481356,0.000591978,0.00057693006,0.00052562065,0.001567879,0.0013775397,0.0009697442,0.0012300946],"category_scores_gemma":[0.0020688914,0.00045925338,0.0006821602,0.0006794695,0.0008226607,0.0017119161,0.0011509692,0.0004198766,0.00031084838],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011851906,0.00004440737,0.033653606,0.00005076092,0.00007637599,0.00040103967,0.0004070992,0.93076575,0.0011235783,0.028654702,0.0005185124,0.00418562],"study_design_scores_gemma":[0.00006370092,0.000042633084,0.004498093,0.0000134655465,0.000029561817,0.00009164539,0.00010694371,0.9716077,0.00016833594,0.022180824,0.0011762345,0.0000207807],"about_ca_topic_score_codex":0.026513875,"about_ca_topic_score_gemma":0.016496513,"teacher_disagreement_score":0.026513875,"about_ca_system_score_codex":0.0010168784,"about_ca_system_score_gemma":0.00071454706,"threshold_uncertainty_score":0.052719116},"labels":[],"label_agreement":null},{"id":"W1980150229","doi":"10.1086/500543","title":"Enhanced Small-Scale Faraday Rotation in the Galactic Spiral Arms","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Spiral galaxy; Galactic plane; Astrophysics; Spiral (railway); Milky Way; Rotation (mathematics); Interstellar medium; Faraday effect; Supernova; Galaxy; Astronomy; Geometry","score_opus":0.005946784565416517,"score_gpt":0.2145846316772848,"score_spread":0.20863784711186828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980150229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99956733,0.00004596862,0.000094469666,0.000007215404,4.531891e-7,4.9481685e-7,0.000061742314,0.000003942145,0.00021828763],"genre_scores_gemma":[0.99982375,0.000020644924,0.00002697453,0.0000012802751,0.0000019465756,4.9809506e-7,0.0000818385,0.0000011092344,0.00004208244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993217,0.000009940669,0.0000038822704,0.0000229209,0.000012793002,0.000018318106],"domain_scores_gemma":[0.9996026,0.000088829016,0.00017018379,0.000034438104,0.000042470903,0.00006157244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012581266,0.00012672991,0.00011749157,0.000719183,0.00010858014,0.0004158153,0.00008675863,0.00009426753,0.00065546925],"category_scores_gemma":[0.0009496115,0.000100525176,0.00009114167,0.0004906953,0.00024879567,0.0002038794,0.00022593944,0.00008080188,0.00012547216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020383956,0.000013259104,0.96541524,0.000015409076,0.00007299368,0.00013756992,0.00024615758,0.0019482261,0.02146996,0.00044643148,0.00014661753,0.009884195],"study_design_scores_gemma":[0.0000019259448,0.0000123669915,0.9984794,9.465715e-7,0.0000057371717,0.00004698914,0.000026328697,0.0008602969,0.0003533617,0.00010127223,0.00010906553,0.000002344157],"about_ca_topic_score_codex":0.0019960173,"about_ca_topic_score_gemma":0.0022839492,"teacher_disagreement_score":0.0019960173,"about_ca_system_score_codex":0.00021790001,"about_ca_system_score_gemma":0.000060628157,"threshold_uncertainty_score":0.003968835},"labels":[],"label_agreement":null},{"id":"W1980195182","doi":"10.1088/0004-637x/725/1/91","title":"SIMULATIONS OF THE SUNYAEV-ZEL'DOVICH POWER SPECTRUM WITH ACTIVE GALACTIC NUCLEUS FEEDBACK","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":204,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Active galactic nucleus; Astrophysics; Galaxy cluster; Cosmic microwave background; Intracluster medium; South Pole Telescope; Galaxy; Redshift; Radiative cooling; Cosmic background radiation; Spectral line; Astronomy","score_opus":0.0043387808082997244,"score_gpt":0.20267690880927475,"score_spread":0.19833812800097503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980195182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98733073,0.00006008393,0.0037961684,0.00024372313,0.00002296016,0.000017453582,0.00056465564,0.0001586457,0.007805606],"genre_scores_gemma":[0.9963708,0.000044530883,0.002253064,0.000052260806,0.000011180322,0.000019820893,0.0004007363,0.000050212253,0.00079733855],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999006,0.000026138692,0.00000480051,0.000014813952,0.000021327392,0.000032395892],"domain_scores_gemma":[0.99898416,0.0005519853,0.00014018187,0.000055364995,0.00010020792,0.00016817013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003287218,0.00038277218,0.00037742846,0.00040090331,0.00035828393,0.00056449743,0.00094951387,0.0005280043,0.002156652],"category_scores_gemma":[0.0019508296,0.00020973326,0.0003782715,0.00048593915,0.00052001985,0.0004493011,0.0005991983,0.00060837995,0.00013676417],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001630372,0.00008933598,0.015581224,0.00003193707,0.00004596772,0.00017558526,0.00011297651,0.97106767,0.0018929507,0.0075949817,0.0009146639,0.0023297286],"study_design_scores_gemma":[0.000050013172,0.000020651594,0.0023532547,0.0000031835461,0.0000058092387,0.000011623548,0.00002947776,0.9957071,0.00042730093,0.0011787725,0.0002072338,0.0000056446956],"about_ca_topic_score_codex":0.019922558,"about_ca_topic_score_gemma":0.013252688,"teacher_disagreement_score":0.019922558,"about_ca_system_score_codex":0.0007081949,"about_ca_system_score_gemma":0.000552057,"threshold_uncertainty_score":0.039613187},"labels":[],"label_agreement":null},{"id":"W1980411230","doi":"10.1088/0004-637x/768/1/16","title":"MAGNETOHYDRODYNAMIC SIMULATION-DRIVEN KINEMATIC MEAN FIELD MODEL OF THE SOLAR CYCLE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Université de Montréal","funders":"European Commission","keywords":"Dynamo; Physics; Differential rotation; Solar dynamo; Magnetohydrodynamics; Meridional flow; Convection zone; Dipole model of the Earth's magnetic field; Mechanics; Turbulence; Dynamo theory; Magnetic field; Solar rotation; Solar cycle; Computational physics; Convection; Classical mechanics; Astrophysics; Interplanetary magnetic field; Zonal and meridional; Solar physics; Atmospheric sciences; Solar wind; Stars","score_opus":0.005940801531578652,"score_gpt":0.21447618218109907,"score_spread":0.20853538064952043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980411230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8280676,0.00027360686,0.13677573,0.000715163,0.000117468066,0.000115850664,0.0024284455,0.00075231737,0.03075386],"genre_scores_gemma":[0.9810659,0.00010537492,0.015387439,0.00005586288,0.000025198495,0.00014415946,0.0005310409,0.000062469146,0.0026226314],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999337,0.0000214419,0.0000035207697,0.0000141871315,0.000013096101,0.0000139918175],"domain_scores_gemma":[0.9997918,0.00006545685,0.00003499602,0.000023258832,0.000048634727,0.000035869172],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016343495,0.0003288798,0.00046623635,0.00032771862,0.00038701316,0.0006895136,0.0011164955,0.0006015581,0.001782613],"category_scores_gemma":[0.0007120055,0.00024559183,0.00045314964,0.00044068965,0.00044767908,0.00042395463,0.00044327948,0.0005053961,0.00018149077],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004228086,0.00001697257,0.0014179896,0.000009770389,0.000014564419,0.000036139187,0.000031861953,0.9906007,0.0008635735,0.005835827,0.00021355017,0.000916754],"study_design_scores_gemma":[0.000022449718,0.0000095573305,0.00026055158,0.0000011230534,0.0000033508172,0.0000073382726,0.0000053704234,0.9981647,0.00013710541,0.0010477713,0.00033707576,0.0000036108308],"about_ca_topic_score_codex":0.015589018,"about_ca_topic_score_gemma":0.00717213,"teacher_disagreement_score":0.015589018,"about_ca_system_score_codex":0.0008068044,"about_ca_system_score_gemma":0.0009962906,"threshold_uncertainty_score":0.030996561},"labels":[],"label_agreement":null},{"id":"W1980414829","doi":"10.1088/0004-637x/731/2/93","title":"STAR CLUSTERS IN THE TIDAL TAILS OF INTERACTING GALAXIES: CLUSTER POPULATIONS ACROSS A VARIETY OF TAIL ENVIRONMENTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; University of Manitoba","funders":"","keywords":"Star cluster; Galaxy; Spiral galaxy; Tidal force; Galaxy cluster; Star formation; Cluster (spacecraft); Luminosity; Population; Hubble space telescope","score_opus":0.02091112986566493,"score_gpt":0.24481709733375331,"score_spread":0.22390596746808838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980414829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998018,0.000018873885,0.00004812249,0.0000016576683,1.1933243e-7,0.0000010352145,0.00004051798,0.0000025319632,0.000085332635],"genre_scores_gemma":[0.99959,0.000018209908,0.000092285736,0.0000037622337,7.5397384e-7,0.0000012862617,0.00019089745,0.0000020405614,0.000100920384],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997794,0.000026525362,0.000017435352,0.000064280975,0.000040141964,0.0000721899],"domain_scores_gemma":[0.9989766,0.00016668806,0.00025962404,0.00013930218,0.00013748836,0.00032023175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031842882,0.00016893426,0.0002576647,0.0015128821,0.0006401876,0.0006625437,0.00030938312,0.00019963222,0.0010919966],"category_scores_gemma":[0.0010368417,0.00015801513,0.00017362855,0.0009782256,0.00040194442,0.00048007062,0.0010020474,0.0001687483,0.00021107477],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007900308,0.000018734461,0.99422354,0.0000036169504,0.000018704792,0.000041271844,0.0004109705,0.000079959806,0.0028910006,0.00003935953,0.000018373803,0.002175439],"study_design_scores_gemma":[0.0000023307055,0.00004017521,0.9985971,0.0000018240314,0.000012701014,0.00010835708,0.00030657678,0.00022440251,0.0005345861,0.000047385896,0.00011965758,0.0000049740447],"about_ca_topic_score_codex":0.0068560205,"about_ca_topic_score_gemma":0.013550431,"teacher_disagreement_score":0.0068560205,"about_ca_system_score_codex":0.00024795026,"about_ca_system_score_gemma":0.00015549053,"threshold_uncertainty_score":0.013632238},"labels":[],"label_agreement":null},{"id":"W1980437607","doi":"10.1086/322393","title":"Constraints on Warm Dark Matter from Cosmological Reionization","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":174,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Reionization; Astrophysics; Redshift; Quasar; Dark matter; Halo; Lyman limit; Galaxy; Supermassive black hole; Dark Ages; Intergalactic medium","score_opus":0.009771148309492213,"score_gpt":0.21419692485015526,"score_spread":0.20442577654066305,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980437607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9850542,0.00042130437,0.0082911905,0.00021159316,0.0000068008208,0.0000034859008,0.000076029544,0.000076094686,0.005859424],"genre_scores_gemma":[0.9989467,0.00010252294,0.0005961914,0.000022422635,0.000009272662,0.0000016081539,0.000056920428,0.000010041927,0.00025439367],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988675,0.000028077393,0.0000056380695,0.000018236902,0.000026219821,0.000035150337],"domain_scores_gemma":[0.99845195,0.00051100523,0.00058913126,0.0001965383,0.00006343,0.00018791233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043303357,0.00061886857,0.0003085898,0.00048174473,0.00032664748,0.0008649086,0.00059077435,0.00032851784,0.0017916971],"category_scores_gemma":[0.0023832335,0.00022454243,0.00034289522,0.0003033483,0.00056614325,0.0010770592,0.0011292691,0.000606199,0.0002687415],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004387366,0.00015436248,0.4181904,0.00022384724,0.00047156014,0.0021079732,0.001041395,0.24580137,0.051716574,0.23076741,0.00200012,0.047086205],"study_design_scores_gemma":[0.0000683541,0.00012506353,0.24157149,0.00008047954,0.00013217633,0.00056480593,0.0003384811,0.50983655,0.010084758,0.23195867,0.0051474376,0.00009171579],"about_ca_topic_score_codex":0.0027964292,"about_ca_topic_score_gemma":0.002607305,"teacher_disagreement_score":0.0027964292,"about_ca_system_score_codex":0.00049752614,"about_ca_system_score_gemma":0.00017695593,"threshold_uncertainty_score":0.0059937835},"labels":[],"label_agreement":null},{"id":"W1980473364","doi":"10.1088/0004-637x/744/1/33","title":"PULSED GAMMA RAYS FROM THE ORIGINAL MILLISECOND AND BLACK WIDOW PULSARS: A CASE FOR CAUSTIC RADIO EMISSION?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Millisecond pulsar; Radio telescope; Gamma ray; Caustic (mathematics); Telescope; Gamma-ray astronomy; Millisecond","score_opus":0.026060264284978454,"score_gpt":0.3041894875477375,"score_spread":0.2781292232627591,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980473364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958405,0.0009498796,0.0010791728,0.00025232404,0.000019593106,0.0000049470104,0.00004074486,0.000023687277,0.0017891881],"genre_scores_gemma":[0.99875104,0.00031868872,0.0005099267,0.000077193385,0.000041383235,0.0000029246582,0.00006652671,0.000009067606,0.00022314802],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984014,0.000019593725,0.000015860614,0.000043520602,0.000034849036,0.00004608064],"domain_scores_gemma":[0.9991035,0.00024541502,0.0003361452,0.00018214528,0.000053610092,0.00007927926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041825225,0.00021149278,0.00021503714,0.0006569386,0.00041323397,0.0013632936,0.00041210966,0.00086191396,0.0011004689],"category_scores_gemma":[0.0018847891,0.00018514557,0.00017937346,0.0005935653,0.00089480914,0.00088250753,0.0008872895,0.00061001617,0.0003551326],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065325527,0.00011797621,0.87776655,0.000086920794,0.00009723236,0.02543655,0.0028036751,0.00019721624,0.038193453,0.0043356884,0.00068310136,0.049628388],"study_design_scores_gemma":[0.00007447689,0.00060555525,0.7909403,0.000112954294,0.00016045044,0.15423106,0.00333913,0.0014810772,0.020558098,0.009161409,0.019280724,0.000054811953],"about_ca_topic_score_codex":0.0003871069,"about_ca_topic_score_gemma":0.00054146454,"teacher_disagreement_score":0.0013632936,"about_ca_system_score_codex":0.0001674647,"about_ca_system_score_gemma":0.00008692317,"threshold_uncertainty_score":0.003681481},"labels":[],"label_agreement":null},{"id":"W1980507920","doi":"10.1086/323777","title":"Constraints on Thermal Emission Models of Anomalous X‐Ray Pulsars","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; McGill University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Magnetar; Astrophysics; Neutron star; Pulsar; Radiative transfer; Magnetic dipole; RADIUS; Thermal; Magnetic field; Computational physics; Optics","score_opus":0.01802048102645889,"score_gpt":0.3060857016284861,"score_spread":0.2880652206020272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980507920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9485544,0.00042226506,0.044031218,0.00016041122,0.000015499674,0.000020234384,0.0001399967,0.00020372393,0.0064522205],"genre_scores_gemma":[0.9970464,0.00018454118,0.0020073561,0.000021798862,0.000017939277,0.000020595233,0.00013301679,0.00005069484,0.00051766937],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997197,0.00006285064,0.00001752725,0.00006299724,0.00006056843,0.000076388074],"domain_scores_gemma":[0.99875724,0.0006146935,0.0002760456,0.00015158557,0.00009027907,0.000110135705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006489884,0.00093724317,0.00038533923,0.00052016386,0.00036631356,0.0014153591,0.0013315337,0.00070750376,0.0013854125],"category_scores_gemma":[0.002533426,0.00067900796,0.0006378742,0.00031963357,0.00081056805,0.0011842444,0.0012780062,0.0004319044,0.00029363393],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072497857,0.00013273022,0.09835393,0.00020858903,0.00019872372,0.0011443391,0.0004840862,0.71797884,0.069349155,0.09306025,0.00074818556,0.01761614],"study_design_scores_gemma":[0.00009172894,0.000109425695,0.021136869,0.000017192886,0.000044773813,0.00035523783,0.00008199022,0.9389619,0.0060597914,0.032316104,0.0007902799,0.000034662786],"about_ca_topic_score_codex":0.0010002214,"about_ca_topic_score_gemma":0.00047307016,"teacher_disagreement_score":0.0014153591,"about_ca_system_score_codex":0.0004831041,"about_ca_system_score_gemma":0.00023076202,"threshold_uncertainty_score":0.0046346784},"labels":[],"label_agreement":null},{"id":"W1980659773","doi":"10.1088/0004-637x/692/2/1609","title":"DISK MASSES IN THE EMBEDDED AND T TAURI PHASES OF STELLAR EVOLUTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; T Tauri star; Angular momentum; Stars; Gravitational collapse; Initial mass function; Stellar mass; Gravitation; Stellar evolution; Astronomy; Star formation; Classical mechanics","score_opus":0.008696542216510162,"score_gpt":0.24890731357023213,"score_spread":0.24021077135372196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980659773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940164,0.00033998024,0.001899955,0.000028531671,0.000027934919,0.000004640429,0.0010196558,0.000105919695,0.0025569627],"genre_scores_gemma":[0.9952632,0.0001387042,0.0025143789,0.000012983394,0.0000073589435,0.0000075773655,0.000915866,0.000030207137,0.0011096363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997365,0.0000027750455,0.0000025867598,0.000010427258,0.0000044708336,0.0000059828812],"domain_scores_gemma":[0.9998609,0.000034034252,0.000059256792,0.000015419497,0.0000092052605,0.00002125104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000057021767,0.00011454419,0.0000796184,0.00045847654,0.000114434595,0.0002909484,0.00017001793,0.00019519485,0.0019562554],"category_scores_gemma":[0.0005917484,0.000062160594,0.00017362657,0.0003032861,0.00016045506,0.00018777003,0.00024232201,0.00014151576,0.0003776509],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015301331,0.000100234,0.6278212,0.00024015436,0.00022653663,0.00073026627,0.0012677249,0.083170965,0.15798423,0.016618075,0.007127313,0.103183165],"study_design_scores_gemma":[0.000031588188,0.00021629821,0.8890528,0.000021092055,0.000033446027,0.0008664859,0.00031308772,0.080753244,0.0135650085,0.004773365,0.010348995,0.000024532024],"about_ca_topic_score_codex":0.001611599,"about_ca_topic_score_gemma":0.0024264304,"teacher_disagreement_score":0.0019562554,"about_ca_system_score_codex":0.00017985866,"about_ca_system_score_gemma":0.00007499905,"threshold_uncertainty_score":0.0065443516},"labels":[],"label_agreement":null},{"id":"W1980699413","doi":"10.1088/0004-637x/725/1/4","title":"VLBI OBSERVATIONS OF THE TYPE I b/c SUPERNOVA 2009bb","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Very-long-baseline interferometry; Astrophysics; Ejecta; Supernova; Light curve; Astronomy; Outflow; RADIUS; Luminosity; Type II supernova; Galaxy","score_opus":0.01737867861569696,"score_gpt":0.23547127010887242,"score_spread":0.21809259149317545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980699413","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9768022,0.0009080174,0.003924437,0.00017141218,0.00004527172,0.00007532292,0.0047128014,0.00023587771,0.013124737],"genre_scores_gemma":[0.9766618,0.0005911232,0.009223842,0.00020783175,0.00004571753,0.000046289224,0.010560171,0.000056026955,0.002607171],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997689,0.000017836246,0.00001123881,0.00005366565,0.00008121158,0.00006727741],"domain_scores_gemma":[0.9995523,0.000029176863,0.000106334206,0.000053284133,0.000081767066,0.00017717628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050223566,0.00023285039,0.00027589974,0.0010312825,0.0007604209,0.00053423207,0.0003873546,0.00042948147,0.00077558646],"category_scores_gemma":[0.0005209436,0.00024825588,0.00025212063,0.00060517987,0.00017493688,0.0002595868,0.0006409752,0.0005929588,0.00069489627],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008522596,0.000605706,0.43287444,0.00019678839,0.0002767478,0.0012322968,0.0007337995,0.0015138933,0.493591,0.0017422726,0.008883942,0.05749684],"study_design_scores_gemma":[0.000045385535,0.00024795154,0.9643242,0.000028544808,0.000067687164,0.0012398467,0.000101655925,0.0014900508,0.012806298,0.00035802255,0.019257037,0.0000333421],"about_ca_topic_score_codex":0.010026806,"about_ca_topic_score_gemma":0.022044761,"teacher_disagreement_score":0.010026806,"about_ca_system_score_codex":0.00055686064,"about_ca_system_score_gemma":0.0003397012,"threshold_uncertainty_score":0.01993692},"labels":[],"label_agreement":null},{"id":"W1980848850","doi":"10.1088/0004-637x/760/1/50","title":"THE ORIGIN OF METALS IN THE CIRCUMGALACTIC MEDIUM OF MASSIVE GALAXIES AT<i>z</i>= 3","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Star formation; Supernova; Milky Way; Redshift; RADIUS; Interstellar medium; Galaxy formation and evolution","score_opus":0.012097731843613789,"score_gpt":0.2361548971268523,"score_spread":0.22405716528323852,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980848850","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99851924,0.000051174757,0.0002319599,0.000035786365,0.0000018542037,0.000005256456,0.00018783861,0.000041632404,0.0009252824],"genre_scores_gemma":[0.99903107,0.0000384831,0.0005570441,0.000015083081,0.000002843638,0.000004759192,0.00020016864,0.000016925984,0.00013367388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999527,0.000006599365,0.0000017701243,0.000010580742,0.000008508329,0.000019933414],"domain_scores_gemma":[0.99978226,0.00004161952,0.000053262804,0.000015163418,0.000017608436,0.00009010029],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000118694334,0.00042842462,0.00024462712,0.00040645082,0.00041246237,0.0008616081,0.0007491169,0.00045471042,0.000629147],"category_scores_gemma":[0.00050699775,0.0003050062,0.00045232385,0.0004703494,0.0004562944,0.00035285414,0.0007629734,0.0003786166,0.000109351226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075075706,0.00024079529,0.67563254,0.000102575184,0.0002771291,0.001777931,0.0011059962,0.22430806,0.078302324,0.008870689,0.0010875387,0.0075436784],"study_design_scores_gemma":[0.00034064782,0.00026196655,0.46232322,0.00002324274,0.00016264415,0.00035072924,0.0006537972,0.5159206,0.013643524,0.0037356392,0.0025168883,0.00006707536],"about_ca_topic_score_codex":0.02606738,"about_ca_topic_score_gemma":0.018853392,"teacher_disagreement_score":0.02606738,"about_ca_system_score_codex":0.0010000479,"about_ca_system_score_gemma":0.00035273845,"threshold_uncertainty_score":0.051831305},"labels":[],"label_agreement":null},{"id":"W1980866569","doi":"10.1086/591672","title":"SDSS J142625.71+575218.3: The First Pulsating White Dwarf with a Large Detectable Magnetic Field","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Zeeman effect; Magnetic field; Helium; Spectral line; Envelope (radar); Excited state; Stars","score_opus":0.008828692675678387,"score_gpt":0.20004058947029857,"score_spread":0.1912118967946202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1980866569","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99734086,0.00027072805,0.00023331032,0.000062776235,0.000030572617,0.0000125219085,0.00056222663,0.000043221007,0.0014438231],"genre_scores_gemma":[0.9951007,0.00013753002,0.0012302707,0.00008543522,0.00004216849,0.000008856986,0.0020537998,0.000017039236,0.0013243834],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999826,0.00000527684,0.000010344675,0.000047492103,0.000053868596,0.00005696765],"domain_scores_gemma":[0.9996761,0.0000103145185,0.000101433056,0.00002443947,0.000043656863,0.00014415679],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021949876,0.00043370182,0.00041923966,0.000983881,0.0008237647,0.0005839084,0.00031200633,0.00043635268,0.0011226818],"category_scores_gemma":[0.00020575241,0.00019357553,0.00015641563,0.00069792534,0.00035999276,0.00022176394,0.0005936499,0.00025098975,0.0007862943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089959515,0.00021664762,0.5424654,0.0002757216,0.00016145027,0.015794817,0.00097041635,0.00044281798,0.39266992,0.0014742804,0.006813139,0.037815884],"study_design_scores_gemma":[0.00006690347,0.0004796312,0.91594857,0.000031085623,0.000057725847,0.008918081,0.00042021487,0.0006552037,0.027163798,0.000305599,0.045907192,0.000046016867],"about_ca_topic_score_codex":0.0026147906,"about_ca_topic_score_gemma":0.0077267303,"teacher_disagreement_score":0.0026147906,"about_ca_system_score_codex":0.0003526786,"about_ca_system_score_gemma":0.0002607937,"threshold_uncertainty_score":0.0051991343},"labels":[],"label_agreement":null},{"id":"W1981027143","doi":"10.1086/499267","title":"Skyrmion Stars: Astrophysical Motivations and Implications","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Neutron star; Stars; Equation of state; Strange matter; Neutrino; Nucleon; Skyrmion; Nuclear matter; Astrophysics; RADIUS; Nuclear physics; Quantum chromodynamics; Mean field theory; Particle physics; Condensed matter physics; Quantum mechanics","score_opus":0.010982186808089284,"score_gpt":0.30199578713021175,"score_spread":0.2910136003221225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981027143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95941055,0.0040965923,0.024445789,0.0012970218,0.000062678606,0.000017613698,0.000113093294,0.00015152054,0.010405148],"genre_scores_gemma":[0.9937471,0.0006059075,0.004495711,0.000045365337,0.00006498352,0.000008580677,0.00006235289,0.000028956554,0.0009409186],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999167,0.000039384096,0.0000030069284,0.000012359519,0.00001724638,0.00001125974],"domain_scores_gemma":[0.9993104,0.0002456996,0.00025861937,0.00004394267,0.000058681908,0.00008260762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000511803,0.00042174634,0.0003694787,0.0005913684,0.00053156615,0.0012575717,0.000659371,0.00087951776,0.0017354888],"category_scores_gemma":[0.00304178,0.00017712354,0.00023993838,0.0007076491,0.0013497671,0.0017342444,0.0009166752,0.00060858356,0.00021612574],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000114071045,0.000078773184,0.03755927,0.00019840173,0.00004233888,0.00086200435,0.00049809786,0.20099121,0.0069182445,0.7416788,0.0019621686,0.009096593],"study_design_scores_gemma":[0.000056447618,0.00014191226,0.015081561,0.000061332175,0.00001643459,0.00070738036,0.0004283845,0.5720819,0.0018377574,0.40459985,0.004945812,0.0000412081],"about_ca_topic_score_codex":0.00083832326,"about_ca_topic_score_gemma":0.00080628984,"teacher_disagreement_score":0.0017354888,"about_ca_system_score_codex":0.000495242,"about_ca_system_score_gemma":0.00018567152,"threshold_uncertainty_score":0.005805731},"labels":[],"label_agreement":null},{"id":"W1981143042","doi":"10.1088/0004-637x/702/1/614","title":"<i>ROSSI X-RAY TIMING EXPLORER</i>MONITORING OF THE ANOMALOUS X-RAY PULSAR 1E 1048.1 – 5937: LONG-TERM VARIABILITY AND THE 2007 MARCH EVENT","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Flare; Physics; Astrophysics; Glitch; Pulsar; Flux (metallurgy); Static timing analysis; Astronomy; Magnetar","score_opus":0.01556004359107086,"score_gpt":0.30938022096231954,"score_spread":0.29382017737124866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981143042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993494,0.0002289205,0.0004228633,0.00017891366,0.000014787993,0.000021072105,0.0026287397,0.00009687725,0.0029139456],"genre_scores_gemma":[0.98983115,0.00020067325,0.002695013,0.00010924992,0.00005563813,0.000018557075,0.006199656,0.000031537547,0.0008585878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999076,0.0000080956015,0.000010375951,0.00002106894,0.00003367112,0.000019189196],"domain_scores_gemma":[0.9995529,0.000027727183,0.00023607089,0.000033897326,0.0000739013,0.00007549886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002200337,0.00016652032,0.00014653911,0.00094444765,0.0002041899,0.00032540076,0.00022114613,0.00023096717,0.00070327404],"category_scores_gemma":[0.0004075978,0.000056248547,0.0001216162,0.00056851655,0.00013353622,0.00015388634,0.00035828547,0.00022827148,0.0002122216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029835777,0.00009734804,0.8692684,0.0000767305,0.00009841038,0.0018754477,0.0002748868,0.00062478747,0.088298365,0.00037403684,0.0047893976,0.0339238],"study_design_scores_gemma":[0.000005254165,0.00006685626,0.99178183,0.000009218771,0.000014739212,0.0007850964,0.00004815517,0.00053741445,0.0038363223,0.00004716804,0.0028605592,0.0000074413706],"about_ca_topic_score_codex":0.005031179,"about_ca_topic_score_gemma":0.01738468,"teacher_disagreement_score":0.005031179,"about_ca_system_score_codex":0.00024544576,"about_ca_system_score_gemma":0.00014626801,"threshold_uncertainty_score":0.010003746},"labels":[],"label_agreement":null},{"id":"W1981166332","doi":"10.1086/501160","title":"The Galaxy Hosts and Large‐Scale Environments of Short‐Hard Gamma‐Ray Bursts","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Lawrence Livermore National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Conselho Nacional de Desenvolvimento Científico e Tecnológico; U.S. Department of Energy; Consejo Nacional de Investigaciones Científicas y Técnicas; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Gamma-ray burst; Dwarf galaxy; Supernova; Redshift","score_opus":0.005666287197634294,"score_gpt":0.20516631651115932,"score_spread":0.19950002931352503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981166332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99915385,0.00015189835,0.000054394375,0.000012719178,0.000001382433,0.0000016201184,0.000059801983,0.000010323769,0.00055399066],"genre_scores_gemma":[0.9996126,0.000066237975,0.00006316453,0.000007593435,0.0000049364653,0.0000014984464,0.000105639134,0.0000033804843,0.00013490477],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998048,0.000022751085,0.00001756998,0.00005851374,0.00002905197,0.00006736392],"domain_scores_gemma":[0.9990477,0.00011094341,0.00045494412,0.000078477635,0.000057967463,0.0002498921],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020148714,0.00023281355,0.0002513933,0.0021092321,0.0005146421,0.0015285726,0.00032934512,0.00033102196,0.0017809429],"category_scores_gemma":[0.00050886685,0.00024746847,0.00016493548,0.0008296311,0.000566742,0.0005690522,0.000942356,0.00026746624,0.00045607195],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023542704,0.000036109726,0.9578722,0.000022524124,0.000035203946,0.00035101984,0.00057732954,0.00014038284,0.036032975,0.00033036547,0.00011583489,0.0042507],"study_design_scores_gemma":[0.0000038585617,0.000033583143,0.9979819,0.000002903521,0.000013752623,0.0003558359,0.00037902727,0.00011827614,0.000804557,0.00006927045,0.00023283125,0.0000041460726],"about_ca_topic_score_codex":0.001960631,"about_ca_topic_score_gemma":0.0023046941,"teacher_disagreement_score":0.0021092321,"about_ca_system_score_codex":0.0002712914,"about_ca_system_score_gemma":0.00009034809,"threshold_uncertainty_score":0.0059579015},"labels":[],"label_agreement":null},{"id":"W1981205029","doi":"10.1088/0004-637x/761/1/12","title":"NEW NEUTRINO MASS BOUNDS FROM SDSS-III DATA RELEASE 8 PHOTOMETRIC LUMINOUS GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"Lawrence Berkeley National Laboratory; Science and Technology Facilities Council; College of Engineering, Michigan State University; York University; Office of Science; Johns Hopkins University; Ohio State University; Vanderbilt University; Yale University; New Mexico State University; University of Portsmouth; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Neutrino; Astrophysics; CMB cold spot; Cosmic microwave background; Redshift; Galaxy; Photometric redshift; Observational cosmology; Hubble's law; Astronomy; Particle physics; Anisotropy","score_opus":0.018087320113731205,"score_gpt":0.2641859054584298,"score_spread":0.24609858534469858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981205029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83875066,0.008418157,0.0779475,0.0007199583,0.0002670332,0.00013487335,0.048748802,0.0028907738,0.022122234],"genre_scores_gemma":[0.92524713,0.00091243815,0.026624665,0.00024483318,0.00015691455,0.00011381317,0.045156974,0.00023838264,0.0013048124],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9974597,0.00040800823,0.00027288496,0.00060255785,0.0009486055,0.00030826402],"domain_scores_gemma":[0.9927746,0.0037132292,0.0012736253,0.0012099914,0.00079125486,0.0002372126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003428851,0.0009653866,0.0007781761,0.0028824937,0.00044554574,0.0023113063,0.0010951478,0.00081981526,0.002378067],"category_scores_gemma":[0.0149119245,0.00041107205,0.0009533491,0.0022502611,0.00039263515,0.0011756143,0.002096586,0.0009795345,0.00076674385],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016689602,0.000255841,0.7372615,0.00070637197,0.0008492477,0.00046893157,0.00085356244,0.0653543,0.025076652,0.021161746,0.0185141,0.12782879],"study_design_scores_gemma":[0.00031571466,0.00030436114,0.64509535,0.00042060518,0.0004600491,0.0008004747,0.0004940452,0.15824404,0.044772293,0.03347038,0.11535477,0.0002679323],"about_ca_topic_score_codex":0.008268219,"about_ca_topic_score_gemma":0.009853154,"teacher_disagreement_score":0.008268219,"about_ca_system_score_codex":0.0012035558,"about_ca_system_score_gemma":0.00030488087,"threshold_uncertainty_score":0.0181337},"labels":[],"label_agreement":null},{"id":"W1981219670","doi":"10.1086/429123","title":"A Survey of Unidentified EGRET Sources at Very High Energies","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Egret; Physics; Astrophysics; Observatory; Telescope; Flux (metallurgy); Astronomy; Gamma ray","score_opus":0.011137881805552512,"score_gpt":0.21630936826869665,"score_spread":0.20517148646314415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981219670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99484813,0.00055896677,0.0010038203,0.000051105824,0.0000053061963,0.000020033858,0.0012570152,0.00007593404,0.0021797442],"genre_scores_gemma":[0.98639756,0.0008016758,0.0031041095,0.00017864995,0.00003545819,0.000031718264,0.0062695076,0.000049928058,0.0031313566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994235,0.000077265395,0.00005145179,0.00012329678,0.00022597266,0.000098479235],"domain_scores_gemma":[0.9971718,0.00034094258,0.0013855393,0.00035641002,0.00040062648,0.00034468411],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060156756,0.00033696726,0.00039547583,0.0040023476,0.00046854437,0.0008364086,0.00055899814,0.00037224093,0.0013806091],"category_scores_gemma":[0.0014258919,0.00026327797,0.00019757742,0.0026586636,0.00026019884,0.00043225515,0.0009630678,0.00026246594,0.0010846861],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015544612,0.00008328282,0.957865,0.0000738601,0.000066660636,0.0013586234,0.0006340744,0.00018254768,0.009860005,0.0004951836,0.0016116314,0.027613692],"study_design_scores_gemma":[0.0000056345284,0.00003996506,0.99294347,0.000012577531,0.000022017131,0.0006812623,0.00011901623,0.00018716419,0.001378704,0.000066293185,0.0045369305,0.0000070176557],"about_ca_topic_score_codex":0.0033621981,"about_ca_topic_score_gemma":0.006303582,"teacher_disagreement_score":0.0040023476,"about_ca_system_score_codex":0.00030364486,"about_ca_system_score_gemma":0.00038831646,"threshold_uncertainty_score":0.006685257},"labels":[],"label_agreement":null},{"id":"W1981238210","doi":"10.1088/0004-637x/780/2/163","title":"A MERGER SHOCK IN A2034","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Astrophysics; Cold front; Physics; Shock (circulatory); Mach number; Ram pressure; Core (optical fiber); Leading edge; Shock wave; Spectrograph; Front (military); Galaxy cluster; Enhanced Data Rates for GSM Evolution; Galaxy; Astronomy; Spectral line; Mechanics; Star formation; Optics; Meteorology","score_opus":0.00625698971848793,"score_gpt":0.20291188344548147,"score_spread":0.19665489372699355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981238210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986089,0.000047386682,0.00011847173,0.000032476146,0.000005117903,0.0000046922255,0.00008610663,0.000033007433,0.0010638111],"genre_scores_gemma":[0.9983479,0.000020624519,0.00048110101,0.000037075024,0.000008392578,0.0000061619576,0.0006230014,0.000008483389,0.00046728025],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998568,0.000011447784,0.000004681255,0.000023995048,0.00004364927,0.000059380385],"domain_scores_gemma":[0.999808,0.0000176588,0.000055018885,0.000015702348,0.000023314487,0.00008025962],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012917034,0.0003158507,0.0004130512,0.00081891974,0.0013496232,0.00067872583,0.00049193867,0.0005919571,0.0013634098],"category_scores_gemma":[0.00034274277,0.00027749178,0.0003155936,0.000904932,0.00031137842,0.00028837653,0.0010326992,0.00050030655,0.00040235344],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0044214833,0.00059974985,0.63770366,0.00017939245,0.00036182016,0.01744915,0.0021042272,0.005175606,0.28678837,0.0026359567,0.006119794,0.03646087],"study_design_scores_gemma":[0.000057084246,0.0004608102,0.9809973,0.000012456467,0.000044060413,0.0018091837,0.0005208588,0.00497527,0.005980641,0.00048775016,0.004608832,0.000045689394],"about_ca_topic_score_codex":0.008720803,"about_ca_topic_score_gemma":0.009720513,"teacher_disagreement_score":0.008720803,"about_ca_system_score_codex":0.0008362273,"about_ca_system_score_gemma":0.00027863283,"threshold_uncertainty_score":0.017340124},"labels":[],"label_agreement":null},{"id":"W1981374430","doi":"10.1088/0004-637x/756/1/65","title":"COSMIC MICROWAVE BACKGROUND CONSTRAINTS ON THE DURATION AND TIMING OF REIONIZATION FROM THE SOUTH POLE TELESCOPE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Reionization; Cosmic microwave background; Physics; Astrophysics; Sunyaev–Zel'dovich effect; South Pole Telescope; Cosmic background radiation; Dark Ages; Star formation; Redshift; Astronomy; Galaxy","score_opus":0.023560484415866525,"score_gpt":0.2290837603921672,"score_spread":0.20552327597630068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981374430","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9587376,0.0013240492,0.023103127,0.00044738146,0.000021048258,0.0000150688575,0.0018081364,0.00022685037,0.0143167395],"genre_scores_gemma":[0.9962812,0.00030516562,0.0021445453,0.000054806824,0.000018711318,0.000007586693,0.0009274779,0.000026849342,0.00023365197],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995863,0.0000652609,0.000021066147,0.00014292092,0.0001276117,0.000056836303],"domain_scores_gemma":[0.99633116,0.0017131782,0.0010742975,0.00046838503,0.0002035576,0.00020949011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012368555,0.00047162865,0.00034142734,0.0007476431,0.00029532574,0.0011782,0.00072324637,0.00039161014,0.0023445394],"category_scores_gemma":[0.0062098433,0.0003482955,0.00037887186,0.00078247144,0.00038684517,0.0008834894,0.0008218345,0.0006313548,0.0002841761],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006744767,0.000081634906,0.604523,0.0002790217,0.0003245075,0.0006453984,0.00050637906,0.22089174,0.03739524,0.072437115,0.0040581375,0.058183298],"study_design_scores_gemma":[0.00005651278,0.000112809495,0.7353723,0.0001138442,0.000098116354,0.0002731895,0.00009906448,0.22924565,0.005557364,0.02198179,0.0070266067,0.00006280153],"about_ca_topic_score_codex":0.0074647693,"about_ca_topic_score_gemma":0.006328217,"teacher_disagreement_score":0.0074647693,"about_ca_system_score_codex":0.0010564403,"about_ca_system_score_gemma":0.0002856279,"threshold_uncertainty_score":0.014842629},"labels":[],"label_agreement":null},{"id":"W1981386761","doi":"10.1088/0004-637x/796/2/88","title":"THE STABLE K0 GIANT STAR β GEM","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Absolute magnitude; Photosphere; Radial velocity; Giant star; Luminosity; Astronomy; Stars; Spectral line","score_opus":0.005675612258167728,"score_gpt":0.19218273217881462,"score_spread":0.1865071199206469,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981386761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991303,0.00006519227,0.000048146932,0.000010426058,0.0000024205008,0.0000020149055,0.000114375514,0.000005795271,0.00062135066],"genre_scores_gemma":[0.99920565,0.000036792244,0.000108875705,0.000019501378,0.0000026909447,0.000001344165,0.00032903274,0.000003087768,0.00029305863],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999646,0.00000283117,0.000002849394,0.000012134231,0.000007236537,0.000010327535],"domain_scores_gemma":[0.99989104,0.0000067812157,0.00002225794,0.000010582239,0.000014600746,0.000054778055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110826346,0.00020098059,0.00017508423,0.00035542285,0.00048422394,0.0003436348,0.00016213761,0.00014249448,0.0005236554],"category_scores_gemma":[0.0001521801,0.00009915103,0.00011637521,0.00034974757,0.00025378665,0.00021865177,0.0003962281,0.00016181312,0.00039925592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009383803,0.00011442806,0.81685627,0.00012542201,0.000063924665,0.001649342,0.0010026334,0.0003578352,0.1602375,0.0005371092,0.0008830784,0.017234078],"study_design_scores_gemma":[0.000019211788,0.00037429744,0.9889369,0.000010935215,0.000025254622,0.0015830399,0.00050584885,0.0004143314,0.0043956833,0.00014553186,0.0035796,0.000009344309],"about_ca_topic_score_codex":0.0018326577,"about_ca_topic_score_gemma":0.0017359094,"teacher_disagreement_score":0.0018326577,"about_ca_system_score_codex":0.00018929585,"about_ca_system_score_gemma":0.000106950676,"threshold_uncertainty_score":0.0036439896},"labels":[],"label_agreement":null},{"id":"W1981432914","doi":"10.1088/0004-637x/801/1/66","title":"BROADBAND X-RAY IMAGING AND SPECTROSCOPY OF THE CRAB NEBULA AND PULSAR WITH<i>NuSTAR</i>","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Crab Nebula; Pulsar; Nebula; Spectroscopy; Torus; Crab Pulsar; Spectral index; Angular diameter; Broadband","score_opus":0.008403690280499386,"score_gpt":0.2772241410246771,"score_spread":0.2688204507441777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981432914","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99477404,0.000343258,0.001271252,0.00003868671,0.000005826538,0.000006452946,0.0002402485,0.000088905595,0.0032313077],"genre_scores_gemma":[0.9928798,0.00018952937,0.005252481,0.00006864384,0.000011493427,0.000011761689,0.0005087212,0.000020612171,0.0010570071],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999409,0.000004838896,0.0000034525976,0.00001495019,0.000021437227,0.000014471246],"domain_scores_gemma":[0.99975973,0.000029491852,0.00007788927,0.00003009312,0.000035013556,0.00006773478],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012693103,0.00012514966,0.00014957118,0.0006322436,0.00024337087,0.00021654178,0.00020464306,0.00031211015,0.0013585376],"category_scores_gemma":[0.00026987435,0.00012268756,0.00015227663,0.00045570754,0.00014505908,0.00019602259,0.00036595843,0.00022701175,0.00030570195],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029777395,0.000080690814,0.11844479,0.000082063576,0.00006322463,0.0008516758,0.00022376333,0.0005899378,0.860673,0.00038462097,0.0005376913,0.017770812],"study_design_scores_gemma":[0.000009109404,0.00019403663,0.9530662,0.000018059807,0.000034460692,0.0044947043,0.00013136351,0.0010787778,0.03820998,0.00023957495,0.002512537,0.000011302917],"about_ca_topic_score_codex":0.00051253726,"about_ca_topic_score_gemma":0.0015393052,"teacher_disagreement_score":0.0013585376,"about_ca_system_score_codex":0.00010838319,"about_ca_system_score_gemma":0.000057040153,"threshold_uncertainty_score":0.0045447946},"labels":[],"label_agreement":null},{"id":"W1981433482","doi":"10.1086/338793","title":"Molecular Cloud Distances via Principal Component Analysis","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Molecular cloud; Principal component analysis; Astrophysics; Cloud computing; Scale (ratio); Calibration; Component (thermodynamics); Dispersion (optics); Statistical physics; Computational physics; Stars; Optics; Statistics; Quantum mechanics","score_opus":0.01018020813163024,"score_gpt":0.22777052282979957,"score_spread":0.21759031469816933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981433482","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.27220985,0.000775364,0.7151352,0.00028306618,0.00011378009,0.00011467598,0.0018335457,0.0038932667,0.005641288],"genre_scores_gemma":[0.7370582,0.00037628177,0.25876567,0.000029590161,0.00008456039,0.0000707146,0.0016957857,0.00034014005,0.001579095],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992029,0.0001364829,0.00004585402,0.0002724073,0.0002590677,0.000083337116],"domain_scores_gemma":[0.9981173,0.00057038484,0.00044973756,0.00029050148,0.00048327626,0.0000887759],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072597887,0.0008127123,0.00042336163,0.0032025,0.00065960013,0.0017922557,0.0006192795,0.00040336847,0.0018999305],"category_scores_gemma":[0.0050685783,0.00030216196,0.00040455072,0.0030331945,0.00036932653,0.0013122882,0.001051686,0.0009668087,0.0013924238],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028032518,0.00014744014,0.06105835,0.0001980757,0.0003951302,0.00014611217,0.0005964927,0.095822826,0.03026821,0.028355112,0.007454763,0.7752771],"study_design_scores_gemma":[0.00003874106,0.000112647314,0.13826652,0.00004610167,0.00011475498,0.00024808812,0.00021001739,0.77997875,0.015546619,0.052851748,0.012372034,0.00021393895],"about_ca_topic_score_codex":0.0076071657,"about_ca_topic_score_gemma":0.005323164,"teacher_disagreement_score":0.0076071657,"about_ca_system_score_codex":0.00050787494,"about_ca_system_score_gemma":0.0006968752,"threshold_uncertainty_score":0.0151257515},"labels":[],"label_agreement":null},{"id":"W1981458776","doi":"10.1088/0004-637x/788/2/147","title":"FIRST EXTRAGALACTIC DETECTION OF SUBMILLIMETER CH ROTATIONAL LINES FROM THE<i>HERSCHEL SPACE OBSERVATORY</i>","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Milky Way; Luminous infrared galaxy; Active galactic nucleus; Star formation; Astronomy; Infrared; Interstellar medium; Space observatory; Submillimeter Array; Spectral line","score_opus":0.013917151437413663,"score_gpt":0.22229580342163408,"score_spread":0.2083786519842204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981458776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9865275,0.0006006686,0.0011653374,0.00017431095,0.00003153831,0.00002182213,0.0015635813,0.00014969031,0.009765658],"genre_scores_gemma":[0.9939965,0.00016800303,0.0028571384,0.00018506084,0.0000377624,0.00000900422,0.0015693192,0.000016778407,0.0011604581],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988496,0.000010848901,0.0000040511786,0.000037214493,0.00003464042,0.000028201],"domain_scores_gemma":[0.9996661,0.00003976449,0.00012569915,0.000049724586,0.000042198775,0.0000765566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018598905,0.00020795527,0.000093666466,0.00048163158,0.00027023687,0.00038884504,0.0002190758,0.0003079714,0.0024190443],"category_scores_gemma":[0.00023373123,0.00012038291,0.00010427397,0.00027767575,0.00016253031,0.00021247813,0.00039848385,0.00032613156,0.00050079916],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023374885,0.00014503239,0.697632,0.00016002858,0.00014764641,0.0010233037,0.00071568385,0.00020737182,0.24720164,0.0010013459,0.004556701,0.046975408],"study_design_scores_gemma":[0.000012906534,0.00008869427,0.9773899,0.000013982333,0.000030861287,0.00036486302,0.000086632725,0.00018761918,0.010103329,0.0001494788,0.011564765,0.000006975546],"about_ca_topic_score_codex":0.0024218871,"about_ca_topic_score_gemma":0.010676836,"teacher_disagreement_score":0.0024218871,"about_ca_system_score_codex":0.0002569523,"about_ca_system_score_gemma":0.00011747387,"threshold_uncertainty_score":0.008092523},"labels":[],"label_agreement":null},{"id":"W1981538234","doi":"10.1088/0004-637x/786/2/79","title":"MAJOR CLUSTER MERGERS AND THE LOCATION OF THE BRIGHTEST CLUSTER GALAXY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Velocity dispersion; Galaxy cluster; Brightest cluster galaxy; Cluster (spacecraft); Abell 2744; Galaxy; Type-cD galaxy; Luminosity","score_opus":0.0038855339088915385,"score_gpt":0.18983434252049416,"score_spread":0.18594880861160262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981538234","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99817646,0.000044285396,0.00090901495,0.000050350623,0.0000030517344,0.0000045618867,0.00012115749,0.000037538142,0.0006536209],"genre_scores_gemma":[0.99869674,0.00001927289,0.0009504089,0.000010275943,0.0000019150036,0.00000389013,0.00014844873,0.000008595933,0.00016048517],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99990666,0.000023941018,0.000003551385,0.00003216201,0.000011844702,0.000021911948],"domain_scores_gemma":[0.9994962,0.000227016,0.0001110575,0.00003586609,0.000038096623,0.00009174112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036539053,0.00026797317,0.00028026252,0.00046112604,0.00046215978,0.0007035,0.00058715645,0.0004622419,0.00086014875],"category_scores_gemma":[0.002261041,0.00033916775,0.00032709434,0.0005116701,0.00051425,0.00044036945,0.00055027875,0.00036414526,0.00008382344],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005619184,0.000111904556,0.20494644,0.000041877334,0.00011007985,0.0002861098,0.00024262725,0.77942866,0.0047459216,0.005110367,0.0006260248,0.003788124],"study_design_scores_gemma":[0.000058528432,0.000056041517,0.0328138,0.000006239039,0.000031974098,0.000053533822,0.00008492568,0.96431136,0.001406794,0.0008759792,0.00028755618,0.000013350732],"about_ca_topic_score_codex":0.027903529,"about_ca_topic_score_gemma":0.02149528,"teacher_disagreement_score":0.027903529,"about_ca_system_score_codex":0.0009871874,"about_ca_system_score_gemma":0.00064999366,"threshold_uncertainty_score":0.05548221},"labels":[],"label_agreement":null},{"id":"W1981568645","doi":"10.1088/0004-637x/692/1/375","title":"HEATING BY ACOUSTIC WAVES OF MULTIPHASE MEDIA","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Dissipation; Mechanics; Physics; Thermal; Acoustic wave; Volume (thermodynamics); Computational physics; Materials science; Thermodynamics; Optics","score_opus":0.006530379366404532,"score_gpt":0.21948718374836615,"score_spread":0.21295680438196163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981568645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9770083,0.00053979165,0.01964551,0.00016875344,0.00003431597,0.000031371164,0.000050331986,0.000050293744,0.002471175],"genre_scores_gemma":[0.99782467,0.00016786667,0.0011199163,0.000019920722,0.000022896947,0.000013577175,0.000018501249,0.000009810032,0.00080297125],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985707,0.000027440397,0.000005248076,0.000024815172,0.000031985637,0.000053470885],"domain_scores_gemma":[0.99906236,0.00042313163,0.00032302973,0.000054545533,0.000047435744,0.000089571404],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028216746,0.0008520911,0.00041934536,0.00082647847,0.0006153381,0.0010550247,0.0005379554,0.0005313278,0.0007719565],"category_scores_gemma":[0.0015331074,0.00042686635,0.0004062798,0.0003892931,0.0015192985,0.0015434185,0.0014593981,0.0005638602,0.00012736896],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073001796,0.00045063975,0.024623968,0.00024290029,0.00017227938,0.0014345853,0.00084611884,0.67778754,0.23426837,0.04611509,0.00047273032,0.01285567],"study_design_scores_gemma":[0.000068578316,0.00010263112,0.0037998117,0.000008955091,0.000024087834,0.00012209211,0.00009519331,0.97631425,0.013554831,0.005528379,0.0003527977,0.000028448067],"about_ca_topic_score_codex":0.0022917402,"about_ca_topic_score_gemma":0.0007504852,"teacher_disagreement_score":0.0022917402,"about_ca_system_score_codex":0.0007392559,"about_ca_system_score_gemma":0.00021493383,"threshold_uncertainty_score":0.0053637624},"labels":[],"label_agreement":null},{"id":"W1981672373","doi":"10.1086/382208","title":"Analysis of a Very Massive DA White Dwarf via the Trigonometric Parallax and Spectroscopic Methods","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Parallax; Effective temperature; Physics; Surface gravity; Astrophysics; Balmer series; RADIUS; Spectral line; Astronomy; Stars; Emission spectrum","score_opus":0.014455344210904882,"score_gpt":0.27672078435359887,"score_spread":0.262265440142694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981672373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94316125,0.00028741575,0.049824893,0.000065373424,0.00002152272,0.000027611533,0.0004876876,0.00056205696,0.0055622603],"genre_scores_gemma":[0.9677513,0.00013042873,0.03014247,0.000020509957,0.00001783427,0.000021628937,0.00044414544,0.000044700057,0.001426988],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998857,0.000012546822,0.0000049086243,0.00003345379,0.00005077234,0.000012597335],"domain_scores_gemma":[0.99968266,0.00005005928,0.000122062695,0.000050521525,0.000055798315,0.0000390035],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019944881,0.0002956779,0.00019814113,0.0016128063,0.000305697,0.00041414457,0.0003053137,0.00021832323,0.0007149844],"category_scores_gemma":[0.0004976082,0.000110166344,0.00018269954,0.0008681882,0.00023781207,0.00021931448,0.0003400043,0.00015953103,0.00058337435],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040094976,0.00006305813,0.18294951,0.00013005889,0.000066228764,0.0015211089,0.0003940222,0.002913513,0.71053046,0.0059614168,0.0005833918,0.09448613],"study_design_scores_gemma":[0.000048073674,0.0005390151,0.6065769,0.000022029808,0.00009009036,0.0047856034,0.00043820174,0.07620575,0.28987858,0.0059236614,0.015420959,0.000071031485],"about_ca_topic_score_codex":0.001427279,"about_ca_topic_score_gemma":0.003011225,"teacher_disagreement_score":0.0016128063,"about_ca_system_score_codex":0.0002522904,"about_ca_system_score_gemma":0.00014650056,"threshold_uncertainty_score":0.002837956},"labels":[],"label_agreement":null},{"id":"W1981736007","doi":"10.1086/340300","title":"Possible Corotation of the Milliarcsecond Radio Structure of the Close Binary HR 1099","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Astronomy; Halo; Sky; RADIUS; Galactic halo; Stellar rotation; Binary star; Stars; Galaxy","score_opus":0.008958169384119476,"score_gpt":0.20534193222569286,"score_spread":0.19638376284157338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981736007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970732,0.00016404717,0.00028230538,0.0000458743,0.000013493193,0.000004143672,0.00010780271,0.000024651883,0.0022844567],"genre_scores_gemma":[0.9992047,0.000023543014,0.00018238902,0.000015448679,0.000010535415,0.0000031810089,0.00020545463,0.0000055986475,0.00034918662],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994266,0.0000047288404,0.000002796964,0.000022811497,0.000012354101,0.000014674651],"domain_scores_gemma":[0.9998172,0.000019685422,0.00007702577,0.000015144349,0.000024955767,0.000046142864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109539185,0.0001111943,0.00019308168,0.00041610422,0.00041673103,0.0005944632,0.0002379924,0.0002979278,0.0016878856],"category_scores_gemma":[0.00041932537,0.00012935893,0.000078600744,0.00023222472,0.0001807549,0.00023080251,0.00035311258,0.00027907308,0.0003717106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006979213,0.00015333526,0.6138693,0.00009744975,0.00005494166,0.0014452449,0.0013574775,0.0009254631,0.35283676,0.0018563985,0.0013022949,0.025403414],"study_design_scores_gemma":[0.000015753207,0.00007705986,0.9922788,0.000010557951,0.0000110332485,0.00029136444,0.00014562909,0.0011262395,0.0035111662,0.00017897812,0.0023452498,0.000008229194],"about_ca_topic_score_codex":0.0022467822,"about_ca_topic_score_gemma":0.0062382044,"teacher_disagreement_score":0.0022467822,"about_ca_system_score_codex":0.0004942853,"about_ca_system_score_gemma":0.0000886136,"threshold_uncertainty_score":0.005646527},"labels":[],"label_agreement":null},{"id":"W1981747069","doi":"10.1086/319428","title":"The Nature of the Radiative Hydrodynamic Instabilities in Radiatively Supported Thomson Atmospheres","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Thermal Radiation and Cooling Technologies","field":"Engineering","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Radiative transfer; Eddington luminosity; Boundary value problem; Instability; Scattering; Electron; Plane (geometry); Boundary (topology)","score_opus":0.004035309487228845,"score_gpt":0.2013639929410936,"score_spread":0.19732868345386476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981747069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9873975,0.00022018756,0.00840981,0.00006279644,0.000006751671,0.000008233786,0.000021852231,0.00004697117,0.00382594],"genre_scores_gemma":[0.99904543,0.000053451786,0.0005699252,0.000004007034,0.000007477085,0.000003319253,0.00001248819,0.0000049501737,0.00029887797],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993384,0.000013747692,0.0000047006743,0.000010001066,0.00001970705,0.000018124088],"domain_scores_gemma":[0.9996902,0.00009112547,0.000111610934,0.000025473682,0.000039804265,0.00004173795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014682402,0.00020024167,0.00015648484,0.00048615277,0.00034894142,0.0007280903,0.00024134251,0.00023627115,0.00044131582],"category_scores_gemma":[0.0011202749,0.0001414657,0.00017543249,0.00016664213,0.0009001177,0.00036687133,0.00046078506,0.0002258087,0.00006660026],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073264836,0.000110546294,0.078492336,0.00014365169,0.00010230405,0.0023690248,0.0015622105,0.2089039,0.36236596,0.3118479,0.0011156857,0.03225383],"study_design_scores_gemma":[0.00009027756,0.00016425039,0.06749776,0.000023661925,0.000033528606,0.0012560836,0.00029497928,0.8083529,0.030081367,0.09083622,0.0012808564,0.00008813987],"about_ca_topic_score_codex":0.0006422422,"about_ca_topic_score_gemma":0.00028446043,"teacher_disagreement_score":0.0007280903,"about_ca_system_score_codex":0.0003665637,"about_ca_system_score_gemma":0.00013562963,"threshold_uncertainty_score":0.0026596785},"labels":[],"label_agreement":null},{"id":"W1981769908","doi":"10.1086/425306","title":"Evolved Galaxies at <i>z</i>  &gt; 1.5 from the Gemini Deep Deep Survey: The Formation Epoch of Massive Stellar Systems","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":215,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Luminous infrared galaxy; Star formation; Elliptical galaxy; Population; Galaxy formation and evolution; Stellar mass; Medicine","score_opus":0.009556101676712647,"score_gpt":0.19978749775992208,"score_spread":0.19023139608320944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981769908","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99474794,0.00029706885,0.00024968394,0.00007746446,0.000006681513,0.000006236038,0.0021653597,0.000045264318,0.0024043242],"genre_scores_gemma":[0.994736,0.00016728116,0.00038131318,0.000033988927,0.00001431904,0.0000033812676,0.0041732127,0.0000054711977,0.00048499228],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999045,0.000006968853,0.000004837571,0.000018996894,0.000022486338,0.000042041553],"domain_scores_gemma":[0.9994444,0.000043992593,0.00024927783,0.00004436183,0.000046911497,0.00017107748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002471683,0.00026404115,0.00013639171,0.0012703466,0.0002820099,0.00055134663,0.00025694986,0.00020729998,0.0015491311],"category_scores_gemma":[0.00049094064,0.000090998816,0.00016464542,0.0008965937,0.00015580042,0.00029619702,0.0004553888,0.00023859562,0.00039210907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008400768,0.000036013258,0.98225635,0.000032098316,0.000024569616,0.0001491766,0.00023503938,0.0002681555,0.004276714,0.00036608253,0.0011848412,0.011086928],"study_design_scores_gemma":[0.0000020277266,0.000014179912,0.99760133,0.0000028358068,0.000010937248,0.00010116377,0.000030301413,0.00020276419,0.000480681,0.000060825834,0.0014913535,0.0000016387679],"about_ca_topic_score_codex":0.004995139,"about_ca_topic_score_gemma":0.013184718,"teacher_disagreement_score":0.004995139,"about_ca_system_score_codex":0.00031391977,"about_ca_system_score_gemma":0.00011518496,"threshold_uncertainty_score":0.009932101},"labels":[],"label_agreement":null},{"id":"W1981863412","doi":"10.1086/427493","title":"Simulations of Relativistic Force‐free Magnetohydrodynamic Turbulence","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Wavenumber; Physics; Turbulence; Magnetohydrodynamic drive; Magnetohydrodynamic turbulence; Magnetohydrodynamics; Anisotropy; Inertia; Magnetic field; Limit (mathematics); K-omega turbulence model; Classical mechanics; K-epsilon turbulence model; Computational physics; Quantum electrodynamics; Statistical physics; Mechanics; Quantum mechanics; Mathematics; Mathematical analysis","score_opus":0.005137011842425051,"score_gpt":0.22092651656856052,"score_spread":0.21578950472613548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981863412","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9864784,0.00016986461,0.0048340503,0.00041889175,0.00006599837,0.0000379871,0.00046143876,0.00022185115,0.0073115365],"genre_scores_gemma":[0.99558157,0.000058690082,0.0032151097,0.00006344743,0.000014603753,0.000043407952,0.00030941973,0.00003044334,0.0006833743],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997912,0.000049967315,0.0000128739275,0.0000292279,0.000039296694,0.00007747138],"domain_scores_gemma":[0.9987381,0.00066100777,0.00012607784,0.000081046106,0.0001562896,0.00023743414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047957964,0.000508557,0.0007657624,0.0003941061,0.0007518514,0.00082800386,0.0013584094,0.0012183888,0.0020059147],"category_scores_gemma":[0.0020914564,0.00036895103,0.00058165076,0.000671147,0.0011310304,0.00057190243,0.0007813929,0.0010766115,0.00015681211],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052425714,0.0002611289,0.0055841324,0.000058001227,0.0000723778,0.0003080723,0.00022293167,0.9825441,0.0025210797,0.0051068785,0.0008514862,0.0019455428],"study_design_scores_gemma":[0.000078145655,0.00006520223,0.0014100461,0.0000064351616,0.000010028099,0.000015338519,0.00005634109,0.9968549,0.00041374433,0.00080936664,0.00026807128,0.000012343079],"about_ca_topic_score_codex":0.018278588,"about_ca_topic_score_gemma":0.008978464,"teacher_disagreement_score":0.018278588,"about_ca_system_score_codex":0.0009203184,"about_ca_system_score_gemma":0.0006901234,"threshold_uncertainty_score":0.03634441},"labels":[],"label_agreement":null},{"id":"W1981926163","doi":"10.1086/429360","title":"A General Relativistic Magnetohydrodynamic Simulation of Jet Formation","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Jet (fluid); Astrophysics; Accretion (finance); Magnetohydrodynamics; Black hole (networking); Magnetohydrodynamic drive; Schwarzschild radius; Mechanics; Astrophysical jet; Shock wave; Magnetic field; Rotational symmetry; Equator; Active galactic nucleus; Astronomy; Galaxy","score_opus":0.011227043270045537,"score_gpt":0.24010183957065476,"score_spread":0.22887479630060922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981926163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98139805,0.00009950033,0.0048271213,0.00039779645,0.000049541915,0.000070231246,0.0008921437,0.00027021626,0.011995447],"genre_scores_gemma":[0.99401927,0.00004183969,0.004329361,0.000086396394,0.000011463473,0.000051362495,0.0005517083,0.000048205155,0.00086044875],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981076,0.000051754752,0.0000062976096,0.000027794866,0.00003089392,0.00007249697],"domain_scores_gemma":[0.9993625,0.00026296265,0.000058107737,0.000040987547,0.000091344584,0.00018398378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038173835,0.00047614967,0.00063767453,0.00032105495,0.00065013027,0.00082200015,0.0015273627,0.0012451676,0.0026548896],"category_scores_gemma":[0.0015856586,0.00040132453,0.00071223045,0.0005282565,0.00085451815,0.0003623848,0.0007692559,0.0010286816,0.00020894245],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031924457,0.00013953308,0.0051529408,0.000033491448,0.00005321108,0.00034667025,0.00012713308,0.9875581,0.0019862226,0.002495565,0.0005668308,0.0012209788],"study_design_scores_gemma":[0.0001584759,0.00007863147,0.0023241537,0.0000044784774,0.000012396585,0.000024241794,0.00005796362,0.99601066,0.00033009122,0.0006142475,0.00037145376,0.0000131629895],"about_ca_topic_score_codex":0.027316276,"about_ca_topic_score_gemma":0.010725621,"teacher_disagreement_score":0.027316276,"about_ca_system_score_codex":0.0011494291,"about_ca_system_score_gemma":0.0010183322,"threshold_uncertainty_score":0.054314554},"labels":[],"label_agreement":null},{"id":"W1981941723","doi":"10.1086/379211","title":"Thermonuclear Stability of Material Accreting onto a Neutron Star","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Thermonuclear fusion; Neutron star; Physics; Accretion (finance); Astrophysics; Neutron; Helium; Nuclear physics; Atomic physics; Plasma","score_opus":0.01445817543080257,"score_gpt":0.2907380338656771,"score_spread":0.2762798584348745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981941723","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99706995,0.00008466945,0.0020541407,0.000007345228,8.634969e-7,0.0000033244153,0.00007103887,0.00001586235,0.0006927256],"genre_scores_gemma":[0.9987801,0.000055504544,0.0006413211,0.0000031292118,0.0000021411452,0.000005080738,0.00016120635,0.000012001971,0.00033959825],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999547,0.0000062835834,0.0000031977797,0.000014009016,0.000012253398,0.000009485024],"domain_scores_gemma":[0.99972135,0.00007804078,0.000104407605,0.00002085915,0.00004198197,0.00003336705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017713943,0.00026849794,0.00018504712,0.00074774004,0.00023410212,0.0004704731,0.00020863429,0.00015273353,0.0009576844],"category_scores_gemma":[0.00070392987,0.00013066285,0.00032298075,0.00025420316,0.0003683894,0.00032351975,0.0003981218,0.00013817342,0.00020361696],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011661972,0.000085290056,0.36412787,0.00018916509,0.00024562425,0.000693487,0.00042295936,0.2613622,0.33148316,0.0059144576,0.00021081186,0.034098763],"study_design_scores_gemma":[0.000021726513,0.0004684668,0.22178948,0.000017048213,0.00006903144,0.00046649648,0.00016687672,0.6965573,0.07653789,0.0031335342,0.0007372354,0.000034901354],"about_ca_topic_score_codex":0.0012349914,"about_ca_topic_score_gemma":0.0010928784,"teacher_disagreement_score":0.0012349914,"about_ca_system_score_codex":0.0004496357,"about_ca_system_score_gemma":0.00013891455,"threshold_uncertainty_score":0.0032624006},"labels":[],"label_agreement":null},{"id":"W1981957979","doi":"10.1086/322977","title":"Molecular Gas in NGC 7129","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Reflection nebula; Outflow; Astrophysics; Young stellar object; Astronomy; Nebula; Star formation; Interstellar medium; Reflection (computer programming); Line (geometry); Stars; Galaxy; Geometry","score_opus":0.007934793970992421,"score_gpt":0.23574670961387803,"score_spread":0.2278119156428856,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1981957979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962268,0.00020734411,0.00007640185,0.000038381888,0.0000045708484,0.0000040404084,0.00020766769,0.00002993195,0.0032049823],"genre_scores_gemma":[0.99873227,0.000084385916,0.00016623824,0.000022052043,0.000003767037,0.0000034434065,0.00047133322,0.0000035995747,0.0005129108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999039,0.000006147718,0.000002861909,0.00002517619,0.000027470907,0.000034460347],"domain_scores_gemma":[0.999866,0.000009240771,0.000031997486,0.000011535123,0.000023791375,0.000057380294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000056272795,0.0001324162,0.00013391122,0.0005312764,0.00075950334,0.00034243282,0.00019058479,0.00021481603,0.0015314062],"category_scores_gemma":[0.00018402482,0.00008746696,0.00007883051,0.00034396735,0.0001829115,0.00018504569,0.00037986191,0.00013454453,0.00058041303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030130244,0.000118352815,0.65591747,0.00009610259,0.00004281948,0.007461223,0.0027255123,0.0024939326,0.29263872,0.0016938545,0.004100117,0.032410588],"study_design_scores_gemma":[0.000017035007,0.000057991616,0.9808956,0.00001649391,0.000011621762,0.0017887837,0.00075066125,0.00089629163,0.003222085,0.0003924891,0.011930172,0.00002072712],"about_ca_topic_score_codex":0.02556523,"about_ca_topic_score_gemma":0.046264846,"teacher_disagreement_score":0.02556523,"about_ca_system_score_codex":0.00051484443,"about_ca_system_score_gemma":0.00019938053,"threshold_uncertainty_score":0.050832868},"labels":[],"label_agreement":null},{"id":"W1982067798","doi":"10.1086/510324","title":"Large‐Scale Parker Winds in Active Galactic Nuclei","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Thermal wind; Galaxy; Active galactic nucleus; Adiabatic process; Photoionization; Kinematics; Scale (ratio); Astronomy; Interstellar medium; Wind speed; Meteorology; Ionization; Classical mechanics; Wind profile power law","score_opus":0.005802678353810599,"score_gpt":0.22185522994304788,"score_spread":0.21605255158923728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982067798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98293686,0.00023104929,0.01333798,0.00013313394,0.0000148298805,0.000025186044,0.00006594142,0.0001181546,0.0031369543],"genre_scores_gemma":[0.99828786,0.00006461986,0.0014082349,0.00001752366,0.0000063212424,0.000009781516,0.000047054873,0.0000076111573,0.0001510237],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99977916,0.0000960175,0.000013086024,0.00003745419,0.00003663618,0.000037707792],"domain_scores_gemma":[0.99798644,0.0009848493,0.0005063241,0.00018451587,0.00014558954,0.00019226545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009323273,0.00045948304,0.0002945561,0.00035405287,0.00037251198,0.00083733164,0.0010242263,0.0007046198,0.0007803828],"category_scores_gemma":[0.006665044,0.00033493573,0.0004413215,0.0002455087,0.00080210733,0.0010492237,0.0008758707,0.00038106737,0.0001568435],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000109370354,0.000053129388,0.1029919,0.000045027846,0.00006844313,0.00046402565,0.000268454,0.8657951,0.0024525756,0.022493739,0.0003562181,0.004902055],"study_design_scores_gemma":[0.000059298898,0.0000745354,0.013895596,0.00001256852,0.000013884275,0.00012841965,0.00008245432,0.9722048,0.0006977892,0.012442195,0.0003662306,0.000022246271],"about_ca_topic_score_codex":0.007460594,"about_ca_topic_score_gemma":0.003551571,"teacher_disagreement_score":0.007460594,"about_ca_system_score_codex":0.00078107906,"about_ca_system_score_gemma":0.00037540318,"threshold_uncertainty_score":0.014834344},"labels":[],"label_agreement":null},{"id":"W1982101692","doi":"10.1088/0004-637x/705/1/446","title":"EXCITATION OF EXTENDED RED EMISSION AND NEAR-INFRARED CONTINUUM RADIATION IN THE INTERSTELLAR MEDIUM","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Black-body radiation; Infrared; Interstellar medium; Excited state; Astrochemistry; Atomic physics; Astrophysics; Photon; Radiation; Astronomy; Galaxy; Optics","score_opus":0.007273827155452943,"score_gpt":0.24092790814651732,"score_spread":0.23365408099106438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982101692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98376113,0.0016185998,0.0024229246,0.00010826305,0.00003170691,0.000011461643,0.000053454536,0.00006526131,0.011927264],"genre_scores_gemma":[0.99708647,0.0004009786,0.0008090379,0.000034074532,0.000009624528,0.000009098694,0.00005730111,0.0000064404453,0.0015869346],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999378,0.000006906205,0.0000012948041,0.000019408351,0.000018753522,0.000015841782],"domain_scores_gemma":[0.9998816,0.00005543503,0.0000195404,0.0000098822065,0.000009189425,0.000024317726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000104802195,0.00018503933,0.00012419398,0.00035702134,0.0002611938,0.0004394695,0.00033225343,0.00028689046,0.002433105],"category_scores_gemma":[0.00019813678,0.00017373322,0.0001605204,0.00019172559,0.0002779891,0.00050384295,0.0006171333,0.00039946052,0.0003442329],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022913661,0.00006091409,0.0062709497,0.00012218182,0.00002214311,0.0012015933,0.00013635035,0.0013139762,0.9791323,0.0045695505,0.00018528815,0.006755641],"study_design_scores_gemma":[0.00015123279,0.00078827085,0.09646154,0.000077360026,0.00006802874,0.0028675236,0.00085182465,0.018795993,0.85909015,0.007845851,0.012933209,0.000069085865],"about_ca_topic_score_codex":0.00026876945,"about_ca_topic_score_gemma":0.0005149051,"teacher_disagreement_score":0.002433105,"about_ca_system_score_codex":0.00027422476,"about_ca_system_score_gemma":0.00011938038,"threshold_uncertainty_score":0.008139491},"labels":[],"label_agreement":null},{"id":"W1982126267","doi":"10.1086/516711","title":"Leo A: A Late-blooming Survivor of the Epoch of Reionization in the Local Group","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":192,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Reionization; Metallicity; Galaxy; Star formation; Local Group; Dwarf galaxy; Galaxy formation and evolution; Billion years; Irregular galaxy","score_opus":0.006367723259762726,"score_gpt":0.20773773014305677,"score_spread":0.20137000688329404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982126267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978434,0.000049006194,0.0001643539,0.00020112515,0.000016604761,0.000020498199,0.00060724665,0.00003197079,0.0010656513],"genre_scores_gemma":[0.9941281,0.00008382764,0.000507091,0.00024659096,0.000028362407,0.000017049031,0.0010839221,0.000021272892,0.00388389],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998883,0.000013207229,0.00000855618,0.000028204644,0.000014235127,0.000047460566],"domain_scores_gemma":[0.99906033,0.000045754878,0.00017805773,0.000102809354,0.00006200702,0.0005510611],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024423163,0.00027882148,0.0002489252,0.0006961159,0.0011480898,0.0006746719,0.00036176865,0.00038909662,0.0030106914],"category_scores_gemma":[0.00049837906,0.00012263985,0.00020718675,0.0004252185,0.00042285945,0.0007333998,0.00096477877,0.0006441231,0.00091083196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011350318,0.0014957851,0.9333345,0.0000478522,0.000059814338,0.009113569,0.0025850113,0.00013403074,0.019400354,0.00074532675,0.0046221823,0.027326552],"study_design_scores_gemma":[0.00004284069,0.0016439651,0.96583253,0.000023764365,0.00003318659,0.01258673,0.0034563038,0.0006064929,0.0030366608,0.00059191714,0.0120974425,0.00004813508],"about_ca_topic_score_codex":0.0059194025,"about_ca_topic_score_gemma":0.010810425,"teacher_disagreement_score":0.0059194025,"about_ca_system_score_codex":0.00031260154,"about_ca_system_score_gemma":0.00024326556,"threshold_uncertainty_score":0.011769891},"labels":[],"label_agreement":null},{"id":"W1982233534","doi":"10.1088/0004-637x/732/1/6","title":"IRAS 15099–5856: REMARKABLE MID-INFRARED SOURCE WITH PROMINENT CRYSTALLINE SILICATE EMISSION EMBEDDED IN THE SUPERNOVA REMNANT MSH15–5<i>2</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Supernova remnant; Silicate; Pulsar; Supernova; H II region; Emission spectrum; Molecular cloud; Outflow; Emission nebula","score_opus":0.017275774201597777,"score_gpt":0.22335557794496103,"score_spread":0.20607980374336324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982233534","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960145,0.00011190141,0.0002474083,0.00003376506,0.000015236532,0.000012390817,0.0003783818,0.00003939412,0.0031470996],"genre_scores_gemma":[0.9976057,0.000045642744,0.00074226264,0.000040611954,0.00002054721,0.000009447908,0.0009261053,0.00000748511,0.00060210435],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991477,0.0000035044727,0.000007764772,0.00002917492,0.00002647696,0.000018345969],"domain_scores_gemma":[0.99979836,0.000007788578,0.00008815399,0.000035626435,0.000011213273,0.00005888389],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009910481,0.00031003862,0.00030516967,0.0005625828,0.00053219433,0.00033951955,0.00049701706,0.0003433028,0.0015263385],"category_scores_gemma":[0.00020042104,0.00018548201,0.00021129203,0.00043292006,0.00024944718,0.00019627619,0.00063284615,0.00024335836,0.00075574074],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007447142,0.00032877704,0.714399,0.00018227422,0.00022794385,0.012823048,0.0005893712,0.0011160556,0.23125762,0.0018599533,0.0045865444,0.03188469],"study_design_scores_gemma":[0.00006395976,0.00029343422,0.9640972,0.000032297423,0.000059200964,0.010521952,0.00015053374,0.0012325222,0.010468952,0.00039758632,0.012661951,0.000020329888],"about_ca_topic_score_codex":0.0011778595,"about_ca_topic_score_gemma":0.002273265,"teacher_disagreement_score":0.0015263385,"about_ca_system_score_codex":0.00025351797,"about_ca_system_score_gemma":0.000094854906,"threshold_uncertainty_score":0.0051060915},"labels":[],"label_agreement":null},{"id":"W1982330764","doi":"10.1088/0004-637x/719/2/1969","title":"THE RISE AND FALL OF PASSIVE DISK GALAXIES: MORPHOLOGICAL EVOLUTION ALONG THE RED SEQUENCE REVEALED BY COSMOS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":204,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Galaxy; Galaxy formation and evolution; Bulge; Population; Astronomy; Star formation","score_opus":0.006785835440793908,"score_gpt":0.2139073949664953,"score_spread":0.20712155952570138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982330764","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984188,0.00021686101,0.000078177174,0.000035987523,0.000001392313,0.0000014786449,0.00022334454,0.0000051619622,0.0010188338],"genre_scores_gemma":[0.99937457,0.00013111133,0.00010432701,0.000010396621,0.0000036543884,0.0000015134535,0.00018673121,0.000003413197,0.00018430018],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986315,0.000028701927,0.0000088203315,0.00005215455,0.000018080393,0.000029090956],"domain_scores_gemma":[0.99913234,0.00012827814,0.00034025137,0.00008634564,0.0001037719,0.00020904446],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041655204,0.00012264265,0.00012673583,0.0012196852,0.0001974567,0.0005958101,0.00018078972,0.0002064081,0.0011808363],"category_scores_gemma":[0.0011544022,0.00014551957,0.00013807965,0.00081445975,0.00040311518,0.0005817389,0.0006177023,0.00022747586,0.0002393934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007511317,0.000007266854,0.9905565,0.000010971764,0.000019747518,0.000050242914,0.00040710077,0.00007886791,0.0036082768,0.00036094588,0.00008368539,0.004741249],"study_design_scores_gemma":[5.0305306e-7,0.0000050111885,0.9996253,0.0000013958553,0.0000022744928,0.000026609108,0.000059505506,0.000048377453,0.000068004556,0.000032024553,0.00013016672,8.3471554e-7],"about_ca_topic_score_codex":0.003169861,"about_ca_topic_score_gemma":0.0042943875,"teacher_disagreement_score":0.003169861,"about_ca_system_score_codex":0.00018333581,"about_ca_system_score_gemma":0.00009613898,"threshold_uncertainty_score":0.0063028336},"labels":[],"label_agreement":null},{"id":"W1982339980","doi":"10.1088/0004-637x/754/2/97","title":"LoCuSS: A DYNAMICAL ANALYSIS OF X-RAY ACTIVE GALACTIC NUCLEI IN LOCAL CLUSTERS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Population; Cluster (spacecraft); Redshift; Luminosity; Velocity dispersion; Galaxy cluster; Astronomy","score_opus":0.005824508343885606,"score_gpt":0.21865572703195701,"score_spread":0.21283121868807142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982339980","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989145,0.000102663755,0.00026178255,0.000010436408,0.0000013851037,0.0000051108495,0.00029501854,0.000012980692,0.00039610403],"genre_scores_gemma":[0.99879164,0.000037637543,0.00034859616,0.0000023768246,0.0000036875279,0.000003987028,0.0005728807,0.0000063013745,0.00023298661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997919,0.000030811334,0.000011956066,0.000078486526,0.00004617181,0.000040779672],"domain_scores_gemma":[0.9992987,0.00009936783,0.00016883897,0.000063962296,0.00009619751,0.00027288953],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002688358,0.0001407797,0.00021051883,0.0019262597,0.00052148965,0.0007073467,0.00034810643,0.00013248908,0.0012590715],"category_scores_gemma":[0.00090718357,0.00010628323,0.0002457122,0.0012683595,0.00032131982,0.00028647148,0.00071128085,0.0001460002,0.00025481856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008727348,0.000022573282,0.9888959,0.000012846802,0.000052706655,0.000118803815,0.00047704633,0.0011834138,0.0028487544,0.00028651016,0.00018538153,0.0058287536],"study_design_scores_gemma":[0.000003533914,0.000032366348,0.9948919,0.0000028025393,0.0000129033415,0.00017018472,0.00050141837,0.0035476547,0.00028289628,0.00010566818,0.00044274644,0.000005940619],"about_ca_topic_score_codex":0.016336044,"about_ca_topic_score_gemma":0.016156193,"teacher_disagreement_score":0.016336044,"about_ca_system_score_codex":0.00052557106,"about_ca_system_score_gemma":0.00030247352,"threshold_uncertainty_score":0.03248191},"labels":[],"label_agreement":null},{"id":"W1982372083","doi":"10.1088/0004-637x/735/2/86","title":"THE NEWFIRM MEDIUM-BAND SURVEY: PHOTOMETRIC CATALOGS, REDSHIFTS, AND THE BIMODAL COLOR DISTRIBUTION OF GALAXIES OUT TO<i>z</i>∼ 3","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":497,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Photometry (optics); Galaxy; Redshift; Telescope; Luminous infrared galaxy; Infrared; Galaxy formation and evolution; Data reduction","score_opus":0.014233073364707631,"score_gpt":0.21808002256745398,"score_spread":0.20384694920274635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982372083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8053096,0.0012098929,0.0063541066,0.00039661597,0.00004961088,0.0002823397,0.15658592,0.0013958871,0.028416054],"genre_scores_gemma":[0.69910526,0.00072927325,0.016070316,0.00031390367,0.00012022163,0.00036844343,0.27102166,0.00032787482,0.011943006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995409,0.00004299873,0.000032428867,0.00012980455,0.00017901485,0.000074975665],"domain_scores_gemma":[0.9984547,0.00007970613,0.0006617516,0.00035375642,0.00022964769,0.00022049836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072812225,0.0003776752,0.0002748058,0.0038218684,0.0003230048,0.0005755929,0.0006955128,0.000219304,0.0055241073],"category_scores_gemma":[0.0014230019,0.00022651665,0.0002540251,0.0032048253,0.00018074473,0.0007955855,0.0011810316,0.00024396657,0.0022421798],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018661845,0.000110516754,0.88011044,0.00017373117,0.00011075921,0.000107398,0.00051351706,0.00046259392,0.0059732147,0.0017521547,0.053560633,0.05693845],"study_design_scores_gemma":[0.000017422897,0.000016816173,0.9720569,0.000017444378,0.00001673487,0.00010704031,0.00007569316,0.0003830575,0.0007728909,0.00014143423,0.026386144,0.000008358537],"about_ca_topic_score_codex":0.018010445,"about_ca_topic_score_gemma":0.040515818,"teacher_disagreement_score":0.018010445,"about_ca_system_score_codex":0.0007107828,"about_ca_system_score_gemma":0.000560317,"threshold_uncertainty_score":0.035811186},"labels":[],"label_agreement":null},{"id":"W1982501656","doi":"10.1088/0004-637x/706/2/1163","title":"X-RAY AND RADIO TIMING OF THE PULSAR IN 3C 58","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Physics; Astrophysics; Offset (computer science); Observatory; Telescope; Supernova; Astronomy; Pulse (music); Radio telescope; Phase (matter); Detector; Optics; Computer science","score_opus":0.011966942594671142,"score_gpt":0.3012509816375448,"score_spread":0.2892840390428737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982501656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99848515,0.00006082378,0.0001584085,0.000014532103,0.0000039664164,0.000003830293,0.00056264363,0.000025031135,0.00068560924],"genre_scores_gemma":[0.9958621,0.00006546849,0.0009305135,0.000015892572,0.00001341175,0.000011940813,0.0026408283,0.000022040234,0.00043771294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999157,0.0000047694657,0.0000053326257,0.000028748009,0.000027354501,0.000018059713],"domain_scores_gemma":[0.99963415,0.000046856992,0.00013638615,0.00004302678,0.000067786554,0.00007169424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019407562,0.00022568538,0.00025357597,0.0012568634,0.00042604926,0.00036082647,0.0003370275,0.00029432087,0.00089189975],"category_scores_gemma":[0.0007840871,0.00013021695,0.00018873501,0.00070575834,0.0002642439,0.00012507544,0.00042269522,0.0003450773,0.00025390863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084362,0.00015860707,0.8584295,0.00009942866,0.00015236781,0.001435252,0.00061482866,0.006613338,0.10043958,0.0006688965,0.0016733046,0.028871221],"study_design_scores_gemma":[0.000020458643,0.00008505692,0.9942789,0.000010298796,0.000023236578,0.000277136,0.000044653196,0.001636366,0.0022223052,0.0000600777,0.0013320281,0.000009468378],"about_ca_topic_score_codex":0.010383296,"about_ca_topic_score_gemma":0.01997737,"teacher_disagreement_score":0.010383296,"about_ca_system_score_codex":0.0004761138,"about_ca_system_score_gemma":0.0001859495,"threshold_uncertainty_score":0.020645738},"labels":[],"label_agreement":null},{"id":"W1982521449","doi":"10.1088/0004-637x/788/2/188","title":"FAINT DWARFS IN NEARBY GROUPS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Galaxy; Sky; Local Group; Astronomy; Satellite galaxy; Redshift; Dwarf galaxy; Luminosity function; Luminosity; Galaxy group; Photometry (optics); Dwarf galaxy problem; Galaxy formation and evolution; Stars","score_opus":0.005747999614167699,"score_gpt":0.20165696660875565,"score_spread":0.19590896699458796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982521449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952077,0.00035200742,0.00046492598,0.0000410704,0.000008725484,0.0000061449728,0.00038393322,0.000038001846,0.0034974692],"genre_scores_gemma":[0.9983334,0.000058249258,0.00028807836,0.00003228696,0.00001137281,0.0000026593873,0.00053602835,0.000006366556,0.0007314669],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996488,0.000028243803,0.000015862266,0.0001775254,0.000073428055,0.00005621463],"domain_scores_gemma":[0.99892247,0.00014892858,0.00036531079,0.0001444476,0.00010938712,0.000309381],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034180903,0.0001332241,0.00036907522,0.0010541807,0.0006090454,0.0007384356,0.0002180351,0.00023123756,0.003351374],"category_scores_gemma":[0.0013734683,0.00010948833,0.00014510764,0.0008128874,0.00058849883,0.00034413132,0.0008867748,0.00016933114,0.0008514078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023934907,0.000031989417,0.96060157,0.000078831676,0.000037482685,0.00022059334,0.001868021,0.00017133457,0.012505501,0.0017865421,0.00089097896,0.021567663],"study_design_scores_gemma":[0.0000060231637,0.00004786391,0.9933831,0.000010144775,0.0000150525175,0.0003916521,0.00054899044,0.0001637346,0.00073550455,0.0010509324,0.0036412773,0.0000056820477],"about_ca_topic_score_codex":0.0038678732,"about_ca_topic_score_gemma":0.0047543244,"teacher_disagreement_score":0.0038678732,"about_ca_system_score_codex":0.00037942923,"about_ca_system_score_gemma":0.00017005927,"threshold_uncertainty_score":0.011211395},"labels":[],"label_agreement":null},{"id":"W1982560564","doi":"10.1086/380432","title":"The Galactic Inner Halo: Searching for White Dwarfs and Measuring the Fundamental Galactic Constant, Θ<sub>0</sub>/<i>R</i><sub>0</sub>","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Galactic halo; Halo; Astrophysics; White dwarf; Constant (computer programming); Physics; Galactic corona; Astronomy; Galactic tide; White (mutation); Milky Way; Galaxy; Stars; Computer science; Chemistry","score_opus":0.014535413394208874,"score_gpt":0.22587723422183897,"score_spread":0.2113418208276301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982560564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976827,0.00009505283,0.00022634924,0.000012716399,0.0000010517757,0.000005481333,0.00014490771,0.000018537788,0.0018131803],"genre_scores_gemma":[0.9972019,0.00012505779,0.0013403641,0.000017726314,0.000006064451,0.000004173716,0.0004280177,0.0000073563374,0.00086937845],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995255,0.0000056579565,0.0000015384356,0.0000117970185,0.000014867274,0.000013517869],"domain_scores_gemma":[0.9998504,0.000008370852,0.00005577448,0.000012043685,0.000022321932,0.00005108089],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011355748,0.0001721853,0.00007122721,0.0008294944,0.0002847657,0.00038340763,0.00020848315,0.00014152845,0.0007684522],"category_scores_gemma":[0.0002461521,0.00010174241,0.000051853272,0.00034098348,0.00021377805,0.00022634651,0.00043919226,0.000085307605,0.0004164034],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008240054,0.000038325732,0.9454373,0.0000185832,0.000017857796,0.00013405934,0.0002642416,0.00014438402,0.034545183,0.0003284733,0.00047061205,0.01851842],"study_design_scores_gemma":[0.000003962762,0.00006070055,0.993986,0.000004507895,0.000014198885,0.00024133007,0.00015451017,0.0002809068,0.0034181026,0.0001513726,0.0016816036,0.0000027118024],"about_ca_topic_score_codex":0.0064016404,"about_ca_topic_score_gemma":0.017239569,"teacher_disagreement_score":0.0064016404,"about_ca_system_score_codex":0.00026538788,"about_ca_system_score_gemma":0.00019187773,"threshold_uncertainty_score":0.012728751},"labels":[],"label_agreement":null},{"id":"W1982626104","doi":"10.1088/0004-637x/763/2/81","title":"THE GREEN BANK TELESCOPE 350 MHz DRIFT-SCAN SURVEY II: DATA ANALYSIS AND THE TIMING OF 10 NEW PULSARS, INCLUDING A RELATIVISTIC BINARY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Killam Trusts; Fonds Québécois de la Recherche sur la Nature et les Technologies; National Radio Astronomy Observatory; National Science Foundation","keywords":"Pulsar; Millisecond pulsar; Telescope; Binary number; White dwarf; Green Bank Telescope; Radio telescope","score_opus":0.045010509740638846,"score_gpt":0.33825392003774724,"score_spread":0.2932434102971084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982626104","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96892226,0.00076393393,0.0055705714,0.00032037386,0.000023794146,0.00010766802,0.019176839,0.0004515587,0.004662988],"genre_scores_gemma":[0.9073173,0.0010496479,0.043686938,0.00033919344,0.000111754096,0.0001453635,0.042803038,0.0002656668,0.0042812545],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996561,0.000055748376,0.000021201125,0.00007821883,0.0001382284,0.000050460472],"domain_scores_gemma":[0.9991966,0.00010312565,0.00019670925,0.00014060832,0.00018541119,0.00017760476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00094153715,0.00028107362,0.00030284142,0.002686125,0.0004435714,0.000531304,0.00038334532,0.00018176925,0.0010617827],"category_scores_gemma":[0.0008040399,0.00032272746,0.00020334648,0.0028051375,0.00020471898,0.00030293613,0.00058778666,0.00031974696,0.0006000014],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003210191,0.00007706597,0.85234654,0.00010445228,0.0001348503,0.0003718826,0.00095970207,0.0020504505,0.03290645,0.0009907179,0.015785528,0.09395127],"study_design_scores_gemma":[0.000027250493,0.00004398814,0.9768034,0.0000146645525,0.000033316977,0.0001879549,0.00009349209,0.0023587353,0.0025868202,0.00017416438,0.017654961,0.000021161468],"about_ca_topic_score_codex":0.03254149,"about_ca_topic_score_gemma":0.05253092,"teacher_disagreement_score":0.03254149,"about_ca_system_score_codex":0.0006532385,"about_ca_system_score_gemma":0.0010774308,"threshold_uncertainty_score":0.06470412},"labels":[],"label_agreement":null},{"id":"W1982684089","doi":"10.1086/344506","title":"Structure of Disk‐dominated Galaxies. I. Bulge/Disk Parameters, Simulations, and Secular Evolution","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":300,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Bulge; Astrophysics; Physics; Galaxy; Surface brightness; Context (archaeology); Type (biology); Thin disk; Astronomy","score_opus":0.004352925989470358,"score_gpt":0.1993198563949029,"score_spread":0.19496693040543256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982684089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98115975,0.0003442475,0.011387887,0.00021379523,0.000020429072,0.000041150823,0.0008108721,0.00017380169,0.0058478946],"genre_scores_gemma":[0.99406034,0.00013992983,0.004402815,0.000052214356,0.000010509741,0.000039072784,0.00046743514,0.00007190801,0.0007557144],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999113,0.000029437928,0.000004189309,0.000018041801,0.000015221768,0.000021778076],"domain_scores_gemma":[0.9995524,0.00015495608,0.00008038309,0.000070593385,0.00007248086,0.000069094815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043180806,0.0004292132,0.00035170492,0.00056522584,0.00053368445,0.0006888479,0.0008971034,0.00087950774,0.0014430329],"category_scores_gemma":[0.0013122908,0.000427776,0.0007216116,0.00040347344,0.00054894417,0.00048821326,0.00047607187,0.0004497103,0.0002858734],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051282535,0.000037035556,0.02271636,0.000024067616,0.00004468031,0.00008707345,0.0000810146,0.96973646,0.0022367272,0.0016843609,0.00040332088,0.0028976281],"study_design_scores_gemma":[0.000016922153,0.000025127185,0.0058676717,0.0000074067143,0.000009923139,0.000025249092,0.00002446533,0.992716,0.0003564799,0.00063608773,0.00030885675,0.0000057211737],"about_ca_topic_score_codex":0.022154117,"about_ca_topic_score_gemma":0.013617024,"teacher_disagreement_score":0.022154117,"about_ca_system_score_codex":0.0013246849,"about_ca_system_score_gemma":0.00047655424,"threshold_uncertainty_score":0.044050336},"labels":[],"label_agreement":null},{"id":"W1982717132","doi":"10.1086/309167","title":"Opacity Sampling in Radiative Acceleration Calculations","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Compute Canada; Université de Moncton","funders":"","keywords":"Physics; Opacity; Radiative transfer; Astrophysics; Stars; Computational physics; Photoionization; Diffusion; Stellar atmosphere; Ion; Ionization; Optics; Quantum mechanics","score_opus":0.025758046086044904,"score_gpt":0.26445114243231466,"score_spread":0.23869309634626976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982717132","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.052598152,0.0001637455,0.93996453,0.0001255333,0.000049665367,0.000071031034,0.00017889705,0.0014643037,0.005384047],"genre_scores_gemma":[0.570334,0.00035884595,0.42473775,0.00007589234,0.000057918,0.00017465335,0.0004109746,0.0011420987,0.0027077787],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9984169,0.00039474556,0.000095181866,0.00009427557,0.0008588094,0.00014005738],"domain_scores_gemma":[0.99074835,0.0057121273,0.0004715038,0.0012452961,0.0016666701,0.00015600471],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023180333,0.00055647513,0.00062617747,0.00091199524,0.0007778332,0.0012388764,0.0014452863,0.00044226402,0.0033488474],"category_scores_gemma":[0.022940971,0.00035590533,0.0006743534,0.000878761,0.0004633302,0.0015223998,0.0011451413,0.00087392045,0.0008885928],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032198956,0.00009590819,0.013500463,0.00023325939,0.00005476736,0.00029001027,0.00067438156,0.67555064,0.016403086,0.11319137,0.0031119762,0.1765721],"study_design_scores_gemma":[0.000024571793,0.000042223513,0.0017964445,0.000026921518,0.000015965416,0.0001097003,0.00006435702,0.9674503,0.009030006,0.01754604,0.0038736002,0.00001994566],"about_ca_topic_score_codex":0.009045454,"about_ca_topic_score_gemma":0.0063242363,"teacher_disagreement_score":0.009045454,"about_ca_system_score_codex":0.0009340063,"about_ca_system_score_gemma":0.0011366495,"threshold_uncertainty_score":0.017985582},"labels":[],"label_agreement":null},{"id":"W1982814811","doi":"10.1086/507666","title":"An Infrared Imaging Study of the Bipolar Proto–Planetary Nebula IRAS 16594−4656","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Bipolar outflow; Physics; Planetary nebula; Asymptotic giant branch; Astrophysics; Torus; Nebula; Infrared; Bipolar nebula; Circumstellar envelope; Astronomy; Reflection nebula; Spectral energy distribution; Envelope (radar); RADIUS; Stars; Star formation; Geometry; Galaxy; Radar","score_opus":0.005913181072314111,"score_gpt":0.22454526139877456,"score_spread":0.21863208032646045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982814811","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960116,0.0004277913,0.00025527138,0.00001443598,0.000004693811,0.000009071516,0.00025084204,0.0000136385715,0.003012495],"genre_scores_gemma":[0.99632144,0.0002675941,0.0012198535,0.00002237578,0.000011086442,0.0000038848325,0.0007936119,0.000007209189,0.0013529042],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999691,0.0000025845243,0.0000014507409,0.000008944974,0.00000977932,0.000008147972],"domain_scores_gemma":[0.9999479,0.0000033563679,0.000014979167,0.0000039692163,0.0000107910855,0.00001889844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000082252,0.00014197001,0.0000908024,0.0009070989,0.000253882,0.00021755978,0.00012617777,0.000121016856,0.0012011669],"category_scores_gemma":[0.00008404387,0.00009270659,0.00009259059,0.00048069775,0.00008870372,0.0001612943,0.00013214842,0.000109844725,0.00031380996],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029974972,0.00024570615,0.06557954,0.00009165061,0.000048980648,0.0010384924,0.00026283407,0.00043693362,0.90541244,0.00039536072,0.0008568875,0.025331408],"study_design_scores_gemma":[0.000011441794,0.00014946949,0.98561907,0.0000069503963,0.000016786315,0.00092028145,0.00011887586,0.000547204,0.009110244,0.000055201857,0.0034401317,0.0000042626575],"about_ca_topic_score_codex":0.002481428,"about_ca_topic_score_gemma":0.002961132,"teacher_disagreement_score":0.002481428,"about_ca_system_score_codex":0.0001451194,"about_ca_system_score_gemma":0.000060598737,"threshold_uncertainty_score":0.0049338937},"labels":[],"label_agreement":null},{"id":"W1982949987","doi":"10.1086/523699","title":"<i>FUSE</i>Observations of Heavy Elements in the Photospheres of Cool DB White Dwarfs","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; White dwarf; Astrophysics; Stars; Spectral line; Astronomy; Stellar atmosphere; Accretion (finance)","score_opus":0.023205173640760177,"score_gpt":0.23389063421037282,"score_spread":0.21068546056961263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982949987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964935,0.00035968772,0.00033750886,0.000014475314,0.0000017112355,0.0000021035432,0.001420118,0.00004360874,0.0013272901],"genre_scores_gemma":[0.99472934,0.00020175861,0.0008388278,0.000026088263,0.000010154726,0.0000025437198,0.003649663,0.000010043438,0.0005315294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999453,0.0000020901173,0.000003581074,0.000012546625,0.00002186979,0.000014683733],"domain_scores_gemma":[0.99987006,0.000011709149,0.00005212607,0.00001139112,0.000021489746,0.000033254335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008782258,0.00019468149,0.00013822548,0.002110439,0.00034828205,0.0003032436,0.00014513668,0.00016034464,0.00051010033],"category_scores_gemma":[0.00014365601,0.00009411556,0.0001661506,0.00071729155,0.0001223126,0.00022458505,0.00026908147,0.00010625911,0.00013997468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030615635,0.000055748624,0.73925126,0.000088183115,0.00014952577,0.00042423533,0.0006299219,0.0013158601,0.22713728,0.00032328017,0.0011507776,0.02916778],"study_design_scores_gemma":[0.0000030350307,0.00003549649,0.9897947,0.000004434305,0.000031543725,0.00037472983,0.0000778223,0.00024854945,0.007519981,0.00012027724,0.0017819444,0.000007446517],"about_ca_topic_score_codex":0.0072449804,"about_ca_topic_score_gemma":0.014289185,"teacher_disagreement_score":0.0072449804,"about_ca_system_score_codex":0.00026611963,"about_ca_system_score_gemma":0.00006882756,"threshold_uncertainty_score":0.014405608},"labels":[],"label_agreement":null},{"id":"W1982961361","doi":"10.1086/533491","title":"Quasar Clustering at 25<i>h</i><sup>−1</sup>kpc from a Complete Sample of Binaries1","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Astrophysics; Physics; Redshift; Galaxy; Sky; Astronomy","score_opus":0.017323202907059392,"score_gpt":0.21051426088763822,"score_spread":0.19319105798057884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982961361","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998295,0.00009570642,0.00030880477,0.000015114315,0.0000010056276,0.000006439451,0.00088522286,0.000012606872,0.00038027365],"genre_scores_gemma":[0.9928276,0.0000752289,0.00082127587,0.000013940082,0.00000998548,0.000009354325,0.0059722573,0.000009427242,0.00026102495],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970764,0.000037026803,0.000024503932,0.00007371338,0.00006888242,0.00008820133],"domain_scores_gemma":[0.99879223,0.00017473266,0.00035435858,0.00019823894,0.00014263834,0.0003378654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042872413,0.00025749527,0.00029194955,0.0019919532,0.0006011285,0.00070524396,0.00049988297,0.00020857144,0.0020702356],"category_scores_gemma":[0.0011131039,0.00019369498,0.00027624296,0.0012323351,0.00028016022,0.00028971967,0.0007838585,0.00021589507,0.0009989172],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013185678,0.00006547672,0.98793876,0.000014333196,0.00007490538,0.00014513546,0.00025162203,0.0004928395,0.003935736,0.00012892314,0.0005807356,0.0062396303],"study_design_scores_gemma":[0.0000035393077,0.000030959032,0.9979956,0.0000018340737,0.000015987885,0.00016332314,0.00006947226,0.0008553693,0.00032694623,0.000059256286,0.0004725411,0.0000051714],"about_ca_topic_score_codex":0.0064700614,"about_ca_topic_score_gemma":0.010410284,"teacher_disagreement_score":0.0064700614,"about_ca_system_score_codex":0.00029952868,"about_ca_system_score_gemma":0.00018692472,"threshold_uncertainty_score":0.0128647685},"labels":[],"label_agreement":null},{"id":"W1982980280","doi":"10.1086/322767","title":"Magnetic Energy of the Intergalactic Medium from Galactic Black Holes","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":153,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Active galactic nucleus; Accretion (finance); Intergalactic travel; Galaxy; Radio galaxy; Galaxy cluster; Astronomy; Magnetic energy; Magnetic field; Redshift","score_opus":0.006245752544201547,"score_gpt":0.19717962574633244,"score_spread":0.1909338732021309,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1982980280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983901,0.00045209326,0.0001308909,0.0000117639465,0.0000035820606,0.0000012254211,0.00017185883,0.0000050062663,0.00083350646],"genre_scores_gemma":[0.9989109,0.00022641143,0.00010660988,0.0000066005987,0.000008192992,0.0000018983908,0.00047719988,0.0000027290253,0.00025940553],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993885,0.000006051885,0.000003064879,0.000012363213,0.00001851513,0.000021170486],"domain_scores_gemma":[0.9997992,0.000053649164,0.00007003092,0.000027879576,0.000024794124,0.000024394833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011568503,0.00022475641,0.00015038317,0.0015676036,0.0001770506,0.00062294997,0.00016485639,0.0001593673,0.0014284499],"category_scores_gemma":[0.00044043892,0.000096394644,0.00013279529,0.0005901648,0.00018002286,0.00029294548,0.00060774834,0.0001362695,0.00023549952],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010253252,0.000094437375,0.48098624,0.00023623757,0.00018894645,0.0015584582,0.000571538,0.0010333349,0.46087807,0.0019603975,0.00033564205,0.051131397],"study_design_scores_gemma":[0.000011178388,0.00006842665,0.9823564,0.000010763272,0.00003047798,0.00051959703,0.00016294324,0.00041503907,0.014937497,0.00048569884,0.0009930031,0.000008880585],"about_ca_topic_score_codex":0.00059356244,"about_ca_topic_score_gemma":0.00074242824,"teacher_disagreement_score":0.0015676036,"about_ca_system_score_codex":0.00021220885,"about_ca_system_score_gemma":0.00004397392,"threshold_uncertainty_score":0.004778683},"labels":[],"label_agreement":null},{"id":"W1983028257","doi":"10.1088/0004-637x/796/2/128","title":"COMPARISON OF ATMOSPHERIC PARAMETERS DETERMINED FROM SPECTROSCOPY AND PHOTOMETRY FOR DA WHITE DWARFS IN THE SLOAN DIGITAL SKY SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Sky; Photometry (optics); White dwarf; Physics; Astrophysics; Spectral line; Instability strip; Astronomy; Spectroscopy; Stars; Cepheid variable","score_opus":0.01985030479055926,"score_gpt":0.2762887794883013,"score_spread":0.256438474697742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983028257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996012,0.000200431,0.0007575842,0.000014629866,0.0000040663267,0.0000054319676,0.0018341731,0.00006279701,0.0011089243],"genre_scores_gemma":[0.9930686,0.00014208574,0.0010474293,0.0000078860485,0.000008080994,0.0000053920226,0.005476656,0.000029438477,0.00021453202],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995629,0.00008675147,0.000038967006,0.000120392535,0.00012435227,0.00006660034],"domain_scores_gemma":[0.9987117,0.00030104452,0.0003484908,0.00021579883,0.000322215,0.000100843536],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000783188,0.00030121222,0.00020533829,0.0026975167,0.00024594215,0.0005008333,0.00018190709,0.00017430466,0.0005606645],"category_scores_gemma":[0.0019684471,0.00012023182,0.0003839226,0.002253445,0.00017627525,0.00031327966,0.00041371956,0.00009909336,0.00023805231],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000099784134,0.000022122427,0.9788244,0.000041897478,0.00014120078,0.000049417507,0.00016604629,0.0033218428,0.0051167784,0.0002473707,0.0004327377,0.011536475],"study_design_scores_gemma":[0.0000026625196,0.000010214017,0.9973896,0.0000027148205,0.000019612342,0.000018965131,0.00005009591,0.0014218634,0.0005561848,0.00003200548,0.00049283396,0.000003362307],"about_ca_topic_score_codex":0.02349016,"about_ca_topic_score_gemma":0.03144446,"teacher_disagreement_score":0.02349016,"about_ca_system_score_codex":0.00061725156,"about_ca_system_score_gemma":0.0003020211,"threshold_uncertainty_score":0.046706855},"labels":[],"label_agreement":null},{"id":"W1983050605","doi":"10.1086/308823","title":"2–45 Micron Infrared Spectroscopy of Carbon‐rich Proto–Planetary Nebulae","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Physics; Astrophysics; Infrared; Radiative transfer; Asymptotic giant branch; Feature (linguistics); Spectroscopy; Astronomy; Stars; Optics","score_opus":0.005746391657869411,"score_gpt":0.21895132631040973,"score_spread":0.2132049346525403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983050605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99652326,0.00033123893,0.00063674344,0.000016846341,0.000003948319,0.000006247329,0.0002848354,0.000045622237,0.002151281],"genre_scores_gemma":[0.9963127,0.00021338768,0.0016403123,0.000031909356,0.0000070225497,0.000009870589,0.0008307451,0.000010491807,0.00094367255],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994993,0.0000028557206,0.0000016964858,0.000019216453,0.000017393582,0.0000088751585],"domain_scores_gemma":[0.9999386,0.000005872717,0.000022195532,0.000006293924,0.000011331991,0.00001578443],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014685329,0.00021904132,0.00008802053,0.00038349576,0.00018076213,0.00019395906,0.00013703661,0.00011614185,0.0005757885],"category_scores_gemma":[0.00012593616,0.00013644765,0.00013429805,0.00016915218,0.00006997245,0.00010433186,0.00015260934,0.00015581987,0.00016901207],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000265635,0.000081689686,0.32775167,0.000090152396,0.00012040781,0.00046881798,0.0002678323,0.0008840211,0.648894,0.00030954988,0.0007169474,0.020149242],"study_design_scores_gemma":[0.000008471477,0.00003336084,0.9886746,0.0000030223064,0.000015673204,0.00023484789,0.000020140307,0.00066332193,0.008597783,0.00004507656,0.0017006705,0.0000030831395],"about_ca_topic_score_codex":0.0019582615,"about_ca_topic_score_gemma":0.002321945,"teacher_disagreement_score":0.0019582615,"about_ca_system_score_codex":0.00023836915,"about_ca_system_score_gemma":0.00006357685,"threshold_uncertainty_score":0.003893733},"labels":[],"label_agreement":null},{"id":"W1983071030","doi":"10.1086/341140","title":"The Variability of the Hg<scp>ii</scp>λ3984 Line of the Mercury‐Manganese Star α Andromedae","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University; Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Mercury (programming language); Manganese; Astrophysics; Spectral line; Rotation period; Magnetic field; Astronomy; Stars; Materials science; Metallurgy","score_opus":0.010684111977097583,"score_gpt":0.20778708804050508,"score_spread":0.1971029760634075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983071030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99933666,0.000027502912,0.000047342455,0.00000920627,9.788389e-7,8.5442235e-7,0.00003474075,0.000004275177,0.0005385001],"genre_scores_gemma":[0.9996784,0.000015992515,0.000056565103,0.0000058544933,0.0000022646548,0.0000011484178,0.000074543204,0.0000020236985,0.0001632217],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999936,0.000010517798,0.000003361434,0.000023907656,0.000014321007,0.000011951223],"domain_scores_gemma":[0.9998398,0.00002277526,0.00006206026,0.00001756845,0.000027988946,0.00002975129],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099065684,0.00009401312,0.0000977675,0.00036806837,0.0002667224,0.00029132146,0.00017238737,0.00024614998,0.00071419374],"category_scores_gemma":[0.0004121839,0.0000954758,0.00006466431,0.00036647197,0.00024050869,0.0001759565,0.00020781472,0.00017818176,0.00032787674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028604476,0.000065812405,0.6470793,0.00004176917,0.00007257732,0.0004868247,0.0007606249,0.00040214532,0.33686823,0.00054751517,0.00036546378,0.013023636],"study_design_scores_gemma":[0.0000054047496,0.000035744528,0.9966169,0.000002368291,0.000006880853,0.00032248037,0.00006623051,0.00031438377,0.0021201414,0.000063858024,0.00044289767,0.0000027719038],"about_ca_topic_score_codex":0.0015588276,"about_ca_topic_score_gemma":0.001931929,"teacher_disagreement_score":0.0015588276,"about_ca_system_score_codex":0.0001965395,"about_ca_system_score_gemma":0.00006459368,"threshold_uncertainty_score":0.0030995607},"labels":[],"label_agreement":null},{"id":"W1983085003","doi":"10.1088/0004-637x/799/2/182","title":"POLARIMETRY WITH THE GEMINI PLANET IMAGER: METHODS, PERFORMANCE AT FIRST LIGHT, AND THE CIRCUMSTELLAR RING AROUND HR 4796A","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":198,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Physics; Polarimetry; Astrophysics; Brightness; Starlight; Linear polarization; Optics; Scattering; Astronomy; Stars","score_opus":0.01054145678714611,"score_gpt":0.2225184401354472,"score_spread":0.2119769833483011,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983085003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.891127,0.0032552464,0.086895496,0.0012457006,0.00007001356,0.000094162875,0.0036606353,0.004411055,0.0092407195],"genre_scores_gemma":[0.7901108,0.0015584361,0.19817759,0.0001635465,0.00013246636,0.00008970408,0.0067574405,0.0008530551,0.0021569957],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99923444,0.00018334229,0.000031232208,0.00016890121,0.00030835462,0.0000737675],"domain_scores_gemma":[0.99907494,0.00018299933,0.00009751775,0.0002910038,0.00027297807,0.00008052388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019880135,0.0005189251,0.00026712578,0.0009786558,0.0005220768,0.0013252124,0.0005335339,0.0004299011,0.0007438797],"category_scores_gemma":[0.0018021548,0.0003224202,0.0002449826,0.0014061534,0.00033723947,0.0013275311,0.00086878485,0.000703674,0.00071613886],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018595161,0.00020005222,0.17441249,0.00027989032,0.00021454101,0.0003811306,0.0009351038,0.016959626,0.34886754,0.0023769843,0.008248769,0.44526428],"study_design_scores_gemma":[0.00018933782,0.00067195453,0.53672385,0.00005730234,0.00019156036,0.0013184001,0.00032045465,0.07632661,0.3496993,0.00239245,0.03188834,0.00022043542],"about_ca_topic_score_codex":0.0034692085,"about_ca_topic_score_gemma":0.0037116953,"teacher_disagreement_score":0.0034692085,"about_ca_system_score_codex":0.0005873767,"about_ca_system_score_gemma":0.00030230227,"threshold_uncertainty_score":0.010513723},"labels":[],"label_agreement":null},{"id":"W1983188969","doi":"10.1086/383523","title":"Three Ly Emitters at <i>z</i> 6: Early GMOS/Gemini Data from the GLARE Project","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Redshift; Galaxy; Astrophysics; Hubble Ultra-Deep Field; Emission spectrum; Spectroscopy; Astronomy; Spectral line; Hubble Deep Field","score_opus":0.02003676366233418,"score_gpt":0.2323957164217115,"score_spread":0.21235895275937733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983188969","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99559456,0.000054622316,0.00032012915,0.000036619167,0.0000017289314,0.0000116014935,0.0020569747,0.00008860245,0.0018351407],"genre_scores_gemma":[0.9814472,0.00008905516,0.0029011741,0.000072186915,0.000013156008,0.000014794025,0.014544512,0.000035063455,0.000883013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998111,0.000013110688,0.00001071458,0.000043135475,0.000069187874,0.000052821313],"domain_scores_gemma":[0.9994597,0.00004650774,0.00016630428,0.00007914055,0.00007201329,0.00017639346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003204953,0.00023517909,0.00016876825,0.0012328711,0.00037540923,0.0004643137,0.0002640593,0.00021043535,0.0010710795],"category_scores_gemma":[0.00030203466,0.000108257685,0.00017494088,0.0008365513,0.00015875955,0.00025713537,0.00059407606,0.00033757897,0.00044802378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048710278,0.00022059058,0.94232994,0.000052596763,0.000055392746,0.00044585005,0.00077158184,0.0004254035,0.023785032,0.000242444,0.0023651014,0.028818961],"study_design_scores_gemma":[0.00001056889,0.00004860044,0.9919418,0.0000032613314,0.000022260854,0.00027779816,0.00009671547,0.00030549697,0.0038126719,0.000051807623,0.003422466,0.0000065606773],"about_ca_topic_score_codex":0.0036165921,"about_ca_topic_score_gemma":0.007830493,"teacher_disagreement_score":0.0036165921,"about_ca_system_score_codex":0.00024201768,"about_ca_system_score_gemma":0.00009002549,"threshold_uncertainty_score":0.0071911216},"labels":[],"label_agreement":null},{"id":"W1983280472","doi":"10.1088/0004-637x/755/2/118","title":"MULTIWAVELENGTH OBSERVATIONS OF THE AGN 1ES 0414+009 WITH VERITAS,<i>FERMI</i>-LAT,<i>SWIFT</i>-XRT, AND MDM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Science; University of Leicester; National Science Foundation; Science Foundation Ireland; U.S. Department of Energy; Smithsonian Institution","keywords":"Physics; BL Lac object; Fermi Gamma-ray Space Telescope; Astrophysics; Crab Nebula; Photon; Flux (metallurgy); Cherenkov radiation; Spectral energy distribution; Extragalactic background light; Gamma ray; Blazar; Galaxy; Detector; Optics","score_opus":0.012994509418613057,"score_gpt":0.2063543372616776,"score_spread":0.19335982784306455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983280472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966583,0.000092212205,0.00024345497,0.000052090807,0.000006558994,0.000008811012,0.00085392094,0.000053561012,0.0020310767],"genre_scores_gemma":[0.98954505,0.00016719596,0.0037248163,0.00007313646,0.000042135343,0.000023858813,0.0048821857,0.00003011165,0.0015114746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974126,0.000018189803,0.000011142971,0.00008223779,0.00010167057,0.000045515095],"domain_scores_gemma":[0.99962354,0.000031342013,0.00015821474,0.00005797295,0.000044688826,0.000084132895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026319717,0.0002567823,0.00029873583,0.0013181957,0.0003403687,0.00047451805,0.00059657154,0.00035145655,0.0011602168],"category_scores_gemma":[0.00042873513,0.00031271597,0.00024165637,0.0007028764,0.000180799,0.0002971542,0.00073442765,0.000266699,0.00034607112],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000873412,0.0004337615,0.79083025,0.000095270494,0.00025693903,0.00088101777,0.0003402841,0.0039122654,0.1470921,0.0012198914,0.0041950475,0.049869757],"study_design_scores_gemma":[0.00009000412,0.00021613136,0.97654414,0.000020115565,0.0000666156,0.0008797751,0.00011120822,0.004558282,0.009039586,0.00029170903,0.008156651,0.00002585031],"about_ca_topic_score_codex":0.004982213,"about_ca_topic_score_gemma":0.022379445,"teacher_disagreement_score":0.004982213,"about_ca_system_score_codex":0.0006734546,"about_ca_system_score_gemma":0.00028543329,"threshold_uncertainty_score":0.009906411},"labels":[],"label_agreement":null},{"id":"W1983313077","doi":"10.1086/426731","title":"21 Years of Timing PSR B1509−58","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Noise (video); Astrophysics; Spectral index; Static timing analysis; Dipole; Spectral line; Astronomy; Computer science","score_opus":0.015591563516116418,"score_gpt":0.32344010861373373,"score_spread":0.30784854509761733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983313077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9531069,0.0009389447,0.02346799,0.00025065008,0.00036347494,0.00008884363,0.009571913,0.00096423173,0.011247111],"genre_scores_gemma":[0.9264684,0.0007085961,0.028767025,0.00018130097,0.00017943584,0.00007834719,0.0388085,0.00017069602,0.004637767],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974734,0.000015516633,0.000023581199,0.000079024605,0.00010487076,0.000029665585],"domain_scores_gemma":[0.99969673,0.00001759095,0.00010514525,0.000050012077,0.00009716355,0.000033485383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035388616,0.00025071183,0.0003054648,0.0011364537,0.00030562008,0.00036339293,0.0003266646,0.00026916075,0.0013157368],"category_scores_gemma":[0.001035947,0.00016468202,0.00021110696,0.00080205686,0.00009982821,0.00027451356,0.00042147667,0.00029992987,0.000971596],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048467872,0.0001339908,0.5134569,0.00023599694,0.0002873925,0.0009569605,0.00051038957,0.019786926,0.0603565,0.0031734682,0.016989112,0.3836278],"study_design_scores_gemma":[0.00005294292,0.00019688884,0.8600208,0.000054617252,0.00011194704,0.0012361294,0.00007518766,0.016527636,0.008080776,0.001180009,0.11240204,0.000061012044],"about_ca_topic_score_codex":0.0064570345,"about_ca_topic_score_gemma":0.01471308,"teacher_disagreement_score":0.0064570345,"about_ca_system_score_codex":0.00029797977,"about_ca_system_score_gemma":0.0002878911,"threshold_uncertainty_score":0.0128389},"labels":[],"label_agreement":null},{"id":"W1983335549","doi":"10.1088/0004-637x/691/2/1235","title":"CONSTRAINTS ON THE PROPERTIES OF THE NEUTRON STAR XTE J1814–338 FROM PULSE-SHAPE MODELS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Calgary","funders":"","keywords":"Physics; Neutron star; Astrophysics; Black-body radiation; RADIUS; Pulsar; Accretion (finance); Equation of state; Isotropy; Star (game theory); Light curve; Radiation; Nuclear physics; Optics","score_opus":0.029478961271190412,"score_gpt":0.21522075084634137,"score_spread":0.18574178957515097,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983335549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.990599,0.00007416002,0.0069806864,0.000060419337,0.0000039923757,0.000013219526,0.00035387967,0.00003983645,0.0018747416],"genre_scores_gemma":[0.9982607,0.00006005323,0.0010994043,0.000013555001,0.000008798287,0.000008720674,0.00038312914,0.000022927235,0.00014284918],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99974936,0.00005267117,0.000026094991,0.000055948894,0.00006753889,0.00004832097],"domain_scores_gemma":[0.99774724,0.0012306909,0.00044698524,0.00032637894,0.00010182898,0.00014683328],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009902989,0.0010271237,0.0007033404,0.0007922295,0.00039873348,0.0014214178,0.00079798704,0.00057400187,0.0016324181],"category_scores_gemma":[0.004884279,0.00066732755,0.0006254272,0.00045032782,0.00039877035,0.001077922,0.00071174465,0.00058185204,0.00036287328],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010415802,0.00018798026,0.4637507,0.00014272131,0.00022322188,0.0009546179,0.00031040478,0.44575906,0.0530473,0.01562677,0.0007692871,0.018186374],"study_design_scores_gemma":[0.00012348963,0.0001566421,0.15599693,0.000028450735,0.00009174249,0.0004949554,0.000111521564,0.8227566,0.0054559866,0.013456946,0.0012657421,0.00006099245],"about_ca_topic_score_codex":0.0015864711,"about_ca_topic_score_gemma":0.00200654,"teacher_disagreement_score":0.0016324181,"about_ca_system_score_codex":0.0007223808,"about_ca_system_score_gemma":0.00036194926,"threshold_uncertainty_score":0.0054609776},"labels":[],"label_agreement":null},{"id":"W1983374839","doi":"10.1086/309378","title":"The Distribution of HCO<sup>+</sup><i>J</i> = 4–3 and HCN<i>J</i> = 4–3 in the Nuclear Region of M82","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Line (geometry); Atomic physics; Astrophysics; Excitation; Mean kinetic temperature; Galaxy; Resolution (logic); Brightness; Astronomy","score_opus":0.006689722272865236,"score_gpt":0.20884203948519772,"score_spread":0.20215231721233248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983374839","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994967,0.0000488866,0.00005532851,0.0000107558,3.275159e-7,5.8120355e-7,0.00008032306,0.000009770599,0.00029724056],"genre_scores_gemma":[0.9995142,0.000021944436,0.00011599222,0.0000081830685,0.000002985156,0.0000021402948,0.0002037539,0.0000042595952,0.00012645095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992037,0.000007909955,0.0000043695172,0.000031762625,0.0000110771825,0.000024439498],"domain_scores_gemma":[0.9996551,0.000058636688,0.00012319545,0.000035912803,0.000060065126,0.00006705531],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008727242,0.0001409046,0.000189862,0.0005812689,0.00024574032,0.00043686692,0.00031917955,0.000301811,0.001223249],"category_scores_gemma":[0.00036662765,0.00021962395,0.0001622513,0.00039155493,0.00035919723,0.00025851044,0.0003295499,0.00014102583,0.00022391067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030844953,0.000033105138,0.8947968,0.000033882126,0.000055884084,0.00033107508,0.00040036847,0.002512485,0.09357376,0.00035789338,0.00035445945,0.0072419085],"study_design_scores_gemma":[0.000003543567,0.000017531083,0.9977787,0.0000024502722,0.0000079572255,0.000072485476,0.00008763703,0.001098325,0.00071320665,0.000049192135,0.00016500049,0.000003938842],"about_ca_topic_score_codex":0.00541617,"about_ca_topic_score_gemma":0.007282659,"teacher_disagreement_score":0.00541617,"about_ca_system_score_codex":0.00032421263,"about_ca_system_score_gemma":0.00008135182,"threshold_uncertainty_score":0.010769308},"labels":[],"label_agreement":null},{"id":"W1983463327","doi":"10.1086/518019","title":"The X‐Ray Structure and Spectrum of the Pulsar Wind Nebula Surrounding PSR B0540−69.3","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Pulsar wind nebula; Nebula; Astrophysics; Pulsar; RADIUS; Astronomy; Spectral index; Observatory; Spectral line; Stars","score_opus":0.007798595886870775,"score_gpt":0.22692871418809216,"score_spread":0.2191301183012214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983463327","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981053,0.00016150647,0.00011621642,0.000016875243,0.000002412089,0.0000025112395,0.00014097219,0.000021002143,0.0014330988],"genre_scores_gemma":[0.998845,0.00009322465,0.0002788296,0.00001870395,0.0000066704083,0.0000028221857,0.0004773673,0.000010079252,0.0002673654],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.0000030404065,0.0000018799066,0.000015555015,0.000016898986,0.000016309681],"domain_scores_gemma":[0.99985814,0.000016046972,0.00005384064,0.000010031812,0.00001935915,0.000042614287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000976758,0.00015908034,0.00015402345,0.00093564246,0.00037499468,0.00034202743,0.00018578095,0.0002063115,0.00080720894],"category_scores_gemma":[0.00021613028,0.00015902528,0.00014386754,0.00074586587,0.00017743526,0.00017687159,0.00035568164,0.00018895017,0.00019588937],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005401858,0.00016382839,0.40318486,0.000105353225,0.00011057878,0.002035683,0.0009799013,0.0021158278,0.5544239,0.00094505097,0.0012551164,0.034139622],"study_design_scores_gemma":[0.000009812863,0.000043507353,0.9948578,0.0000052390196,0.000011314782,0.0004655004,0.000059556776,0.000816345,0.002469385,0.00008659586,0.0011699665,0.0000050545973],"about_ca_topic_score_codex":0.0050322204,"about_ca_topic_score_gemma":0.007198673,"teacher_disagreement_score":0.0050322204,"about_ca_system_score_codex":0.00024608406,"about_ca_system_score_gemma":0.00010003709,"threshold_uncertainty_score":0.010005832},"labels":[],"label_agreement":null},{"id":"W1983464972","doi":"10.1088/0004-637x/732/1/2","title":"ON THE INTERPRETATION OF SUPERNOVA LIGHT ECHO PROFILES AND SPECTRA","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Supernova; Light scattering; Light curve; Spectral line; Echo (communications protocol); Milky Way; Interpretation (philosophy); Galaxy","score_opus":0.012461882626856775,"score_gpt":0.21431643620817692,"score_spread":0.20185455358132015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983464972","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.032984845,0.0034613528,0.7088408,0.004966417,0.0038330473,0.00010628929,0.0019308663,0.0065501677,0.23732628],"genre_scores_gemma":[0.50493956,0.0064152735,0.34185454,0.0012423134,0.001953164,0.00006743369,0.0017011513,0.005421463,0.13640505],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998203,0.000051124774,0.00001800216,0.000026189866,0.000066125736,0.000018308756],"domain_scores_gemma":[0.9989586,0.0004236105,0.00006735167,0.0001701507,0.0003314299,0.000048855385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004958924,0.0007531877,0.00033018042,0.0021277252,0.00067423645,0.0043578986,0.0009198407,0.00083709636,0.045623615],"category_scores_gemma":[0.0047253584,0.00032638008,0.00045917326,0.0014891707,0.0010010793,0.0019757873,0.000814622,0.0010176605,0.00909927],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036618675,0.000049051207,0.0033895965,0.00047402098,0.00006848537,0.0028230508,0.0014488936,0.01995912,0.029815832,0.51998436,0.055722,0.3658994],"study_design_scores_gemma":[0.000039434548,0.000044683962,0.01195644,0.00041084905,0.000079829566,0.0025967006,0.0013152838,0.07122472,0.015333869,0.48511395,0.41178635,0.00009783228],"about_ca_topic_score_codex":0.0026568652,"about_ca_topic_score_gemma":0.0020554163,"teacher_disagreement_score":0.045623615,"about_ca_system_score_codex":0.00043559613,"about_ca_system_score_gemma":0.0002793784,"threshold_uncertainty_score":0.15262628},"labels":[],"label_agreement":null},{"id":"W1983635152","doi":"10.1086/379119","title":"Optimal Weak‐Lensing Skewness Measurements","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Skewness; Weak gravitational lensing; Cosmic microwave background; Physics; Cosmology; Dark matter; Galaxy; Gaussian; Noise (video); Constraint (computer-aided design); COSMIC cancer database; Statistical physics; Astrophysics; Statistics; Redshift; Optics; Computer science; Mathematics; Image (mathematics)","score_opus":0.018878634931495247,"score_gpt":0.25855521402514503,"score_spread":0.23967657909364978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983635152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5067828,0.00048031242,0.4874386,0.00039951823,0.000030282687,0.000051029736,0.0008205889,0.00056327664,0.0034336236],"genre_scores_gemma":[0.90783435,0.00026513136,0.09041255,0.000051954794,0.00003963523,0.000035745725,0.0007912903,0.000085716914,0.0004837492],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99878126,0.00047389144,0.00008125377,0.0001984503,0.00024778367,0.00021738335],"domain_scores_gemma":[0.99408793,0.0033308757,0.00083055143,0.00086180045,0.0006405881,0.00024812066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032177716,0.00079042016,0.000843254,0.0008562596,0.00040426353,0.0010154296,0.0007002068,0.0005710078,0.0018564624],"category_scores_gemma":[0.017056203,0.00047534838,0.000554052,0.0006763464,0.00072899985,0.001637037,0.0013132897,0.0005068975,0.0003175966],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031979731,0.00023774395,0.08578917,0.0005381357,0.00047431877,0.00060382363,0.00029614812,0.47239867,0.094766505,0.110167034,0.0032745383,0.228256],"study_design_scores_gemma":[0.00015365765,0.00023207608,0.04600597,0.000059251142,0.00015941246,0.00029353032,0.00014568186,0.8098673,0.04815898,0.09273974,0.0020481346,0.0001362148],"about_ca_topic_score_codex":0.0024871388,"about_ca_topic_score_gemma":0.0026975267,"teacher_disagreement_score":0.0032177716,"about_ca_system_score_codex":0.0005939827,"about_ca_system_score_gemma":0.0013191766,"threshold_uncertainty_score":0.017017424},"labels":[],"label_agreement":null},{"id":"W1983701437","doi":"10.1086/424906","title":"The Mouse that Soared: High‐Resolution X‐Ray Imaging of the Pulsar‐powered Bow Shock G359.23−0.82","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Pulsar wind nebula; Astronomy; Bow shock (aerodynamics); Radio telescope; Nebula; Shock (circulatory); X-ray pulsar; Shock wave; Stars","score_opus":0.009694176271569576,"score_gpt":0.2775044006818771,"score_spread":0.2678102244103075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983701437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967175,0.00018718274,0.00051121716,0.00007139512,0.0000131827865,0.000010431495,0.00034640337,0.00012898135,0.002013595],"genre_scores_gemma":[0.99570113,0.00015499628,0.0021996202,0.0001311124,0.000019691737,0.000009381434,0.00053665217,0.000037133035,0.0012101962],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999783,9.908903e-7,6.228926e-7,0.000006134213,0.000005676922,0.000008310876],"domain_scores_gemma":[0.99992967,0.000005473852,0.000015487793,0.0000074209543,0.0000057239954,0.00003615983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007599203,0.00015130876,0.00012874855,0.00035354038,0.00014177454,0.00027773264,0.00022463771,0.00020684351,0.001454887],"category_scores_gemma":[0.00009307481,0.00016184027,0.00015697068,0.00028801546,0.00010094476,0.00014615843,0.00029163103,0.00037309836,0.00020662669],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005708207,0.000079827136,0.08181491,0.00010674973,0.00010439608,0.0049573597,0.00037518737,0.00094128057,0.89254194,0.0008480311,0.0028629992,0.014796493],"study_design_scores_gemma":[0.0000553006,0.0002884635,0.96250904,0.00004358605,0.000055034485,0.0046226205,0.00022207134,0.002761599,0.021126006,0.00036434684,0.007930651,0.000021381244],"about_ca_topic_score_codex":0.0010871015,"about_ca_topic_score_gemma":0.0029992256,"teacher_disagreement_score":0.001454887,"about_ca_system_score_codex":0.00012487132,"about_ca_system_score_gemma":0.00009221021,"threshold_uncertainty_score":0.004867077},"labels":[],"label_agreement":null},{"id":"W1983786503","doi":"10.1088/0004-637x/755/2/128","title":"WIND COMPETING AGAINST SETTLING: A COHERENT MODEL OF THE GW VIRGINIS INSTABILITY DOMAIN","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Canadian Space Agency","funders":"","keywords":"Physics; Opacity; Envelope (radar); Astrophysics; Settling; Domain (mathematical analysis); Instability; Enhanced Data Rates for GSM Evolution; Mechanics; Optics; Thermodynamics","score_opus":0.020553448200674927,"score_gpt":0.3034457089814861,"score_spread":0.28289226078081114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983786503","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7797734,0.00088947394,0.11373479,0.0035135758,0.00013872884,0.000115812516,0.000309846,0.00021774569,0.1013067],"genre_scores_gemma":[0.98872656,0.00022116459,0.0036090687,0.00014086475,0.00008489379,0.000056183766,0.000055884408,0.000039743336,0.0070658154],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998677,0.00002957032,0.0000061258593,0.000023887791,0.000030419355,0.000042414118],"domain_scores_gemma":[0.99951744,0.000104316845,0.000103974984,0.000040599312,0.000058661444,0.00017503103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045123877,0.00040984616,0.0006823065,0.0006561739,0.0011460071,0.0025935734,0.0015153347,0.00230792,0.005596014],"category_scores_gemma":[0.0013556663,0.00035535765,0.00084432337,0.00032273913,0.002005384,0.002625316,0.0022254412,0.0010050653,0.0006087718],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007521257,0.000082101265,0.0017516481,0.000034315628,0.000025873043,0.0005970884,0.00029015067,0.18239287,0.00431879,0.8064686,0.0012907464,0.0026725635],"study_design_scores_gemma":[0.000081279744,0.000053081654,0.0007175242,0.000013732552,0.000011458712,0.000097140146,0.000112829606,0.845695,0.0001685105,0.1521129,0.00091444724,0.00002219866],"about_ca_topic_score_codex":0.0033073984,"about_ca_topic_score_gemma":0.0015967633,"teacher_disagreement_score":0.005596014,"about_ca_system_score_codex":0.00085205224,"about_ca_system_score_gemma":0.00080964674,"threshold_uncertainty_score":0.018720508},"labels":[],"label_agreement":null},{"id":"W1983834603","doi":"10.1086/521293","title":"Combining Strong and Weak Gravitational Lensing in Abell 1689","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":299,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Weak gravitational lensing; Galaxy; Redshift; Mass distribution; Gravitational lens; Strong gravitational lensing; Dark matter; Galaxy cluster; Gravitational lensing formalism","score_opus":0.009665047359980592,"score_gpt":0.2310322248819676,"score_spread":0.221367177521987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983834603","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99758387,0.00006935663,0.0012299744,0.000026345579,0.000003127608,0.0000042461497,0.00026395512,0.000076401586,0.0007427364],"genre_scores_gemma":[0.9972811,0.000031344764,0.001954488,0.000008563218,0.0000062434283,0.0000030674998,0.00050557795,0.000020551497,0.00018900752],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998228,0.000018615365,0.0000065334175,0.00004708158,0.000057663834,0.00004734173],"domain_scores_gemma":[0.9997181,0.000026611935,0.000110786874,0.000031247324,0.000031950374,0.00008122705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018622026,0.0004286628,0.0004573937,0.0011568139,0.0003534947,0.00060139445,0.00040855553,0.00025772394,0.0010674471],"category_scores_gemma":[0.0005639744,0.00029772363,0.00036493797,0.0005348139,0.000323299,0.00028205718,0.000758601,0.000249633,0.00033608355],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001689885,0.0001531583,0.53476554,0.00016460315,0.00034267298,0.004280329,0.00053541845,0.037970383,0.36698064,0.00283217,0.0013755986,0.048909687],"study_design_scores_gemma":[0.000033103443,0.00015385539,0.9217923,0.000019008257,0.00006961569,0.00083808793,0.00019289748,0.055311922,0.018424071,0.0010961696,0.0020078043,0.000061088365],"about_ca_topic_score_codex":0.010383506,"about_ca_topic_score_gemma":0.016880946,"teacher_disagreement_score":0.010383506,"about_ca_system_score_codex":0.0006767807,"about_ca_system_score_gemma":0.00024674117,"threshold_uncertainty_score":0.020646155},"labels":[],"label_agreement":null},{"id":"W1983949389","doi":"10.1086/343085","title":"A New ZZ Ceti White Dwarf Pulsator: G30‐20","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; White dwarf; Astrophysics; Light curve; Astronomy; Stars","score_opus":0.01389162774613815,"score_gpt":0.21497479969314184,"score_spread":0.2010831719470037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983949389","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99815506,0.00034510627,0.00026527626,0.00015180832,0.00003126179,0.0000059595814,0.00012126518,0.000029662493,0.0008945308],"genre_scores_gemma":[0.9981014,0.00020730999,0.0005489756,0.00019433262,0.00005640697,0.0000046604414,0.00041519193,0.000008633724,0.0004631785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993443,0.0000030674444,0.0000036120139,0.000025048112,0.000013934102,0.000019961908],"domain_scores_gemma":[0.99981207,0.000019537309,0.000060112154,0.000021505146,0.000008577061,0.00007831845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009113594,0.0002457694,0.00021958459,0.00040502052,0.0003912014,0.00047105917,0.0002815529,0.00051850633,0.00047298337],"category_scores_gemma":[0.0002376695,0.000111900794,0.00013895813,0.0003922216,0.00044549795,0.00030597663,0.0006336591,0.00037387153,0.000255862],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008197755,0.00015785998,0.61108035,0.00018035776,0.00008283754,0.031324822,0.0016659468,0.00021508793,0.30306268,0.0024840664,0.0040416354,0.04488458],"study_design_scores_gemma":[0.00008609013,0.0012578527,0.7738362,0.000025171534,0.00010093398,0.13788635,0.0006797348,0.0009824608,0.03813908,0.0023966106,0.04454438,0.000065092965],"about_ca_topic_score_codex":0.00038587447,"about_ca_topic_score_gemma":0.0007218984,"teacher_disagreement_score":0.00051850633,"about_ca_system_score_codex":0.00013635698,"about_ca_system_score_gemma":0.00008095551,"threshold_uncertainty_score":0.0015823245},"labels":[],"label_agreement":null},{"id":"W1983981351","doi":"10.1086/309531","title":"Highly Polarized Thermal Dust Emission in the Bok Globule CB 068","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Wavelength; Astrophysics; Polarimeter; Polarization (electrochemistry); Turbulence; Magnetic field; Thermal emission; Linear polarization; Polarimetry; Astronomy; Thermal; Protostar; Cosmic dust; Stars; Star formation; Optics; Scattering; Chemistry; Meteorology","score_opus":0.008164116615593553,"score_gpt":0.23101597628927825,"score_spread":0.2228518596736847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1983981351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999554,0.000014243103,0.000053524815,0.000009312553,9.1598594e-7,0.0000018250394,0.000036488254,0.000010122621,0.00031956326],"genre_scores_gemma":[0.99957913,0.000008731408,0.0001815437,0.000012292281,0.0000014734321,0.000002606318,0.00008965065,0.000005253602,0.00011936225],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995494,0.000001790854,0.0000011354824,0.000013844568,0.000008649682,0.000019566953],"domain_scores_gemma":[0.9998704,0.000010365714,0.000019519452,0.000015382748,0.000028811835,0.000055366567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000697387,0.00015024329,0.00020610054,0.00030765802,0.0006179988,0.0003601666,0.0002760263,0.00021067043,0.0005578274],"category_scores_gemma":[0.00013397867,0.00016904011,0.00011147606,0.00020249942,0.00029549302,0.00014308254,0.0004556094,0.00027905765,0.00016161606],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053521415,0.00011338383,0.32801813,0.000043233555,0.000044853652,0.0008940535,0.0012156297,0.00044235078,0.66216624,0.00019445484,0.00039925348,0.005933296],"study_design_scores_gemma":[0.000023800058,0.00006961924,0.9812122,0.0000074795284,0.000019859539,0.00046571664,0.00046127284,0.00078841543,0.015789535,0.00007062655,0.0010798125,0.000011540545],"about_ca_topic_score_codex":0.0060319444,"about_ca_topic_score_gemma":0.008025205,"teacher_disagreement_score":0.0060319444,"about_ca_system_score_codex":0.0003075536,"about_ca_system_score_gemma":0.0001008497,"threshold_uncertainty_score":0.011993647},"labels":[],"label_agreement":null},{"id":"W1984005139","doi":"10.1088/0004-637x/797/2/89","title":"INVESTIGATING BROADBAND VARIABILITY OF THE TeV BLAZAR 1ES 1959+650","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Science Foundation; Science Foundation Ireland; U.S. Department of Energy; Office of Science; Smithsonian Institution","keywords":"Blazar; Physics; Fermi Gamma-ray Space Telescope; Astrophysics; Telescope; Synchrotron; Context (archaeology); Flux (metallurgy); Jet (fluid); BL Lac object; Spectral energy distribution; Gamma ray; Cherenkov Telescope Array; Broadband; Crab Nebula; Astronomy; Cherenkov radiation; Galaxy; Detector; Optics","score_opus":0.0071751570267460495,"score_gpt":0.20810508989565757,"score_spread":0.20092993286891153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984005139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971033,0.00026489515,0.00060537,0.000020841817,0.0000031866637,0.000006179135,0.00034813368,0.000025391028,0.0016226827],"genre_scores_gemma":[0.99884284,0.00011026707,0.00032680464,0.000009166816,0.000007689286,0.0000023728383,0.00053961686,0.0000050500626,0.00015617414],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993086,0.000005834688,0.000004500278,0.000028992441,0.0000122161655,0.000017615284],"domain_scores_gemma":[0.99984574,0.000026784712,0.00007211218,0.000015116818,0.000013186858,0.000027016937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001811151,0.0002073848,0.00017927891,0.0010241922,0.00017850501,0.00041277253,0.00017996535,0.00018822121,0.00063383725],"category_scores_gemma":[0.000357052,0.000107997854,0.00023827984,0.00054554257,0.00014455881,0.00021332684,0.0002898089,0.00017398038,0.00011190133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018919956,0.000074548974,0.9143495,0.00012331133,0.00027076268,0.0007974895,0.00046981598,0.014330334,0.045968655,0.0019531135,0.000552026,0.020921195],"study_design_scores_gemma":[0.000005790217,0.000040736097,0.99315685,0.0000137791685,0.00003308712,0.00014333216,0.00008038511,0.004403774,0.0008608303,0.000223936,0.0010298953,0.000007661557],"about_ca_topic_score_codex":0.006297414,"about_ca_topic_score_gemma":0.007396734,"teacher_disagreement_score":0.006297414,"about_ca_system_score_codex":0.00039351106,"about_ca_system_score_gemma":0.0000874617,"threshold_uncertainty_score":0.012521505},"labels":[],"label_agreement":null},{"id":"W1984152927","doi":"10.1086/427919","title":"Atomic Diffusion and ο Leonis","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Stars; Astrophysics; Hertzsprung–Russell diagram; Astronomy; Stellar evolution","score_opus":0.007222167880072878,"score_gpt":0.2136776677962835,"score_spread":0.20645549991621062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984152927","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.061998196,0.046920873,0.0068225157,0.19231552,0.019075187,0.000060648537,0.0002105011,0.00026655992,0.67232996],"genre_scores_gemma":[0.45869,0.026501931,0.0021312223,0.008954907,0.018949088,0.000067074965,0.00014987552,0.00016938923,0.4843866],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997937,0.00004140448,0.000008713001,0.00007719538,0.000050178318,0.000028776647],"domain_scores_gemma":[0.9995415,0.00019307276,0.000032955024,0.00004174508,0.00012204035,0.000068727546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00080215925,0.00040540233,0.0005196141,0.00075693004,0.0022517082,0.002126864,0.00044604825,0.0016980489,0.010041167],"category_scores_gemma":[0.0025561226,0.00014901585,0.00032904948,0.00045484694,0.0015088689,0.0019102104,0.0013774204,0.0020860843,0.001255472],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037116883,0.0000251046,0.0013125351,0.00012630125,0.00001917274,0.00017670935,0.0009788802,0.00067726115,0.00053940644,0.8651303,0.1019938,0.02898351],"study_design_scores_gemma":[0.00002154553,0.000027633048,0.0025500292,0.00012599997,0.000017140514,0.000423187,0.00037678215,0.0015200548,0.00053634087,0.41203198,0.58234835,0.000020895412],"about_ca_topic_score_codex":0.0019644033,"about_ca_topic_score_gemma":0.0018796675,"teacher_disagreement_score":0.010041167,"about_ca_system_score_codex":0.0018920556,"about_ca_system_score_gemma":0.0005702442,"threshold_uncertainty_score":0.03359109},"labels":[],"label_agreement":null},{"id":"W1984181456","doi":"10.1086/587130","title":"Dynamical Models for Disk Galaxies with Triaxial Halos","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Halo; Astrophysics; Galaxy rotation curve; Bulge; Dynamical friction; Cuspy halo problem; Galaxy; Dark matter halo; Galactic halo","score_opus":0.01204228736087003,"score_gpt":0.20965419548434558,"score_spread":0.19761190812347554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984181456","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8780345,0.0005373808,0.10629499,0.00078134023,0.00006709241,0.00010012941,0.00055098895,0.0003075509,0.013326032],"genre_scores_gemma":[0.98763776,0.00024003038,0.007779188,0.0000722968,0.00003375028,0.00009917471,0.0002450836,0.0000646605,0.0038280408],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998548,0.00005454665,0.000008924559,0.000024615663,0.000022588752,0.0000344306],"domain_scores_gemma":[0.99938357,0.00013094483,0.00015406088,0.00005984683,0.00009753468,0.00017403129],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003808084,0.0004695305,0.0005309899,0.00087571674,0.0007015741,0.0012082338,0.0013631146,0.00097072305,0.0018195282],"category_scores_gemma":[0.0015389345,0.0004413497,0.00083552254,0.00038883172,0.0012609714,0.0012129083,0.0010765914,0.0005523707,0.00033847874],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006292777,0.000039674767,0.0061994754,0.000023339013,0.00004188501,0.00021297675,0.00023161442,0.9352886,0.0019682483,0.053700265,0.00072286034,0.0015081911],"study_design_scores_gemma":[0.00003067283,0.000012269629,0.0008991677,0.0000038117673,0.0000062831577,0.000027717464,0.000029263361,0.99032015,0.000087028304,0.008072841,0.0005005956,0.000010173178],"about_ca_topic_score_codex":0.01616727,"about_ca_topic_score_gemma":0.008656904,"teacher_disagreement_score":0.01616727,"about_ca_system_score_codex":0.0015572713,"about_ca_system_score_gemma":0.00051190646,"threshold_uncertainty_score":0.032146335},"labels":[],"label_agreement":null},{"id":"W1984204014","doi":"10.1088/0004-637x/758/2/108","title":"SUBMILLIMETER LINE SPECTRUM OF THE SEYFERT GALAXY NGC 1068 FROM THE<i>HERSCHEL</i>-SPIRE FOURIER TRANSFORM SPECTROMETER","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Line (geometry); Radiative transfer; Surface brightness; Spectrometer; Emission spectrum; Astronomy; Spectral line; Optics","score_opus":0.011811038319160227,"score_gpt":0.2231606422177385,"score_spread":0.21134960389857826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984204014","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9702495,0.00029655045,0.0016551634,0.0007034857,0.000057306155,0.000017656834,0.012830293,0.00091014936,0.013279986],"genre_scores_gemma":[0.97961754,0.00022743078,0.0033001145,0.00035247815,0.000052397445,0.0000150831265,0.013323151,0.00010792967,0.0030039318],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999386,0.0000053186586,0.0000033087604,0.000021249956,0.000020278861,0.000011245306],"domain_scores_gemma":[0.99975854,0.000043239917,0.00005033433,0.0000380261,0.000041688607,0.00006823861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019481592,0.00020905404,0.00020360317,0.0008453199,0.0002949411,0.00018142416,0.00042221358,0.0004417902,0.005223284],"category_scores_gemma":[0.00022822514,0.00012722476,0.00022703275,0.0005344931,0.0001277749,0.0003126826,0.00022564514,0.0003624477,0.00087745447],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017044856,0.00070469204,0.27143523,0.00033956938,0.0003808256,0.0017905198,0.00054259517,0.0049474505,0.6316443,0.002152004,0.033603866,0.050754327],"study_design_scores_gemma":[0.000057223864,0.00007767778,0.9814694,0.000014886594,0.00004694621,0.00030298918,0.00006881141,0.0026258002,0.01068652,0.00030320193,0.004331306,0.000015171132],"about_ca_topic_score_codex":0.0031122465,"about_ca_topic_score_gemma":0.006243226,"teacher_disagreement_score":0.005223284,"about_ca_system_score_codex":0.00024021855,"about_ca_system_score_gemma":0.00011186602,"threshold_uncertainty_score":0.017473578},"labels":[],"label_agreement":null},{"id":"W1984282591","doi":"10.1088/0004-637x/691/2/1764","title":"THE GROWTH AND MIGRATION OF JOVIAN PLANETS IN EVOLVING PROTOSTELLAR DISKS WITH DEAD ZONES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; McMaster University","funders":"","keywords":"Planetary migration; Planet; Physics; Planetesimal; Accretion (finance); Jovian; Formation and evolution of the Solar System; Protoplanetary disk; Gas giant; Astronomy; Astrophysics; Exoplanet; Nice model; Astrobiology; Uranus; Planetary system; Jupiter mass; Planetary mass; Saturn","score_opus":0.005611147614146017,"score_gpt":0.21283398290904348,"score_spread":0.20722283529489746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984282591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984635,0.000037184207,0.000893307,0.000028960196,0.0000037575926,0.0000032546309,0.000028552893,0.000017660415,0.0005237754],"genre_scores_gemma":[0.9985305,0.000040458475,0.0010680411,0.0000098186,0.0000019993538,0.0000046490095,0.000050120943,0.000009585392,0.00028470776],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999528,0.000007828739,0.000003783637,0.000010753927,0.000008614555,0.000016201873],"domain_scores_gemma":[0.99962425,0.00013854311,0.00009794495,0.000034337572,0.000024479605,0.00008048092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001571883,0.00029861255,0.00024817567,0.0003777573,0.00056132785,0.0007269318,0.0006980504,0.0006493943,0.00074500556],"category_scores_gemma":[0.0014900522,0.0002823257,0.0004153328,0.00025238612,0.00057445123,0.0006362434,0.000766917,0.00037545327,0.000089757275],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028308964,0.00021416877,0.0971364,0.00008355075,0.00010990346,0.0011063977,0.0005783555,0.86788386,0.022047065,0.0041595064,0.0003106427,0.0060870186],"study_design_scores_gemma":[0.000072071176,0.00012168027,0.017218348,0.000010730623,0.00003474392,0.00017788878,0.0002411467,0.97768855,0.002779367,0.0009844224,0.0006550404,0.00001595174],"about_ca_topic_score_codex":0.008500558,"about_ca_topic_score_gemma":0.004866348,"teacher_disagreement_score":0.008500558,"about_ca_system_score_codex":0.0005911441,"about_ca_system_score_gemma":0.00033026826,"threshold_uncertainty_score":0.016902149},"labels":[],"label_agreement":null},{"id":"W1984334130","doi":"10.1086/591726","title":"A Parameter Study of Classical Be Star Disk Models Constrained by Optical Interferometry","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Interferometry; Radiative transfer; Stars; Circumstellar disk; Line (geometry); Optical depth; Star (game theory); Spectroscopy; Be star","score_opus":0.02612636708427688,"score_gpt":0.2538665084474296,"score_spread":0.2277401413631527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984334130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99189574,0.00015720796,0.006029146,0.00009947317,0.0000038852613,0.000011146732,0.0002670795,0.000051114435,0.0014852574],"genre_scores_gemma":[0.9980592,0.000080728605,0.0014080822,0.000016639458,0.000004338948,0.000011126059,0.00023157106,0.000015236669,0.00017309155],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996911,0.00009500388,0.000014986021,0.000096176016,0.00003879871,0.00006384375],"domain_scores_gemma":[0.9976891,0.0014388502,0.0002763022,0.00024434557,0.00017322929,0.00017813263],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00094080844,0.00096038677,0.0007813921,0.00082903367,0.00069664384,0.0012566221,0.0018595939,0.0010349571,0.0009586338],"category_scores_gemma":[0.004848915,0.0004916424,0.00056625117,0.00080423115,0.0010415992,0.0016973837,0.00069162395,0.00080935354,0.00012921679],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000098224715,0.000045990793,0.012148996,0.000027570446,0.000039742394,0.00009669221,0.00010835119,0.98146,0.0008191848,0.003636647,0.00013966662,0.0013789419],"study_design_scores_gemma":[0.000020129855,0.000029747616,0.0027078437,0.000006241728,0.000011616685,0.000028513488,0.000042849148,0.9947813,0.0003265702,0.0018929468,0.00013985221,0.000012350362],"about_ca_topic_score_codex":0.015074157,"about_ca_topic_score_gemma":0.0056338967,"teacher_disagreement_score":0.015074157,"about_ca_system_score_codex":0.0013281975,"about_ca_system_score_gemma":0.00059133884,"threshold_uncertainty_score":0.029972851},"labels":[],"label_agreement":null},{"id":"W1984370115","doi":"10.1088/0004-637x/759/1/54","title":"MAGNETIC FIELDS FROM QCD PHASE TRANSITIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Laurentian University","funders":"","keywords":"Physics; Magnetic helicity; Helicity; Magnetic field; Magnetohydrodynamics; Quantum chromodynamics; Turbulence; Magnetohydrodynamic turbulence; Quantum electrodynamics; Amplitude; Astrophysics; Computational physics; Particle physics; Mechanics; Quantum mechanics","score_opus":0.008739721782857313,"score_gpt":0.2596798783853908,"score_spread":0.2509401566025335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984370115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9567305,0.00044580793,0.025149891,0.0005306457,0.00006112502,0.000035144087,0.000115047886,0.00023552707,0.016696298],"genre_scores_gemma":[0.9983076,0.000078585246,0.00088207505,0.00003249525,0.000017713774,0.000008734966,0.000032619413,0.000013936091,0.0006261835],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999193,0.000026623433,0.0000025202773,0.000008183958,0.000015810083,0.000027558892],"domain_scores_gemma":[0.99968386,0.00010807467,0.000087949426,0.000020437537,0.000033365926,0.00006634745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015451858,0.00034876564,0.0002824926,0.000293754,0.0005804866,0.00092675426,0.00035442825,0.0004544781,0.0012609311],"category_scores_gemma":[0.0013147609,0.00019991718,0.00034453886,0.00019549324,0.0010012229,0.0005895357,0.0007267288,0.0005125722,0.000117297015],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031628777,0.0001110498,0.011464024,0.00014733935,0.000058800186,0.001168128,0.00036546687,0.60674006,0.020879634,0.3513825,0.0016307354,0.005735931],"study_design_scores_gemma":[0.00008372763,0.000042842712,0.0028070759,0.000010448606,0.000011381186,0.0001055607,0.000044141645,0.935424,0.0016721652,0.059143994,0.0006347192,0.000019978148],"about_ca_topic_score_codex":0.005808427,"about_ca_topic_score_gemma":0.001699273,"teacher_disagreement_score":0.005808427,"about_ca_system_score_codex":0.0009869016,"about_ca_system_score_gemma":0.0006415487,"threshold_uncertainty_score":0.011549234},"labels":[],"label_agreement":null},{"id":"W1984397353","doi":"10.1086/375771","title":"The Role of Polycyclic Aromatic Hydrocarbons in Ultraviolet Extinction. I. Probing Small Molecular Polycyclic Aromatic Hydrocarbons","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Ultraviolet; Extinction (optical mineralogy); Spectral line; Absorption (acoustics); Stars; Infrared; Absorption spectroscopy; Interstellar medium; Astrochemistry","score_opus":0.006484146813377233,"score_gpt":0.210803318905622,"score_spread":0.2043191720922448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984397353","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9758354,0.011775485,0.0035247153,0.0002056773,0.000025245557,0.000015579999,0.00027417898,0.000055658606,0.008288019],"genre_scores_gemma":[0.99379337,0.00292077,0.0016345176,0.00007212183,0.00003048686,0.0000046857294,0.00019098786,0.0000052006076,0.0013479987],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.999902,0.000013292768,0.000004382591,0.000022973913,0.000034763263,0.000022541333],"domain_scores_gemma":[0.999663,0.00008136398,0.00011977001,0.000021064026,0.00006467672,0.00005011313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019804762,0.00026515874,0.000109049346,0.000615047,0.00024357864,0.00041164848,0.00024862163,0.00027972678,0.0018085592],"category_scores_gemma":[0.0003828545,0.00013757787,0.00013721967,0.00043138757,0.00038155064,0.0005893958,0.0003146467,0.0003265939,0.00027133382],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037218668,0.00014026635,0.34515527,0.00038191557,0.00007634255,0.00047164326,0.00018695625,0.0013208472,0.5679209,0.00220817,0.00030473224,0.08146078],"study_design_scores_gemma":[0.0000117907175,0.00045066242,0.80668366,0.000058919362,0.000081308324,0.0011843324,0.00020263839,0.0032373278,0.17746586,0.00298613,0.007619226,0.000018338],"about_ca_topic_score_codex":0.0014396481,"about_ca_topic_score_gemma":0.0016382673,"teacher_disagreement_score":0.0018085592,"about_ca_system_score_codex":0.0002150478,"about_ca_system_score_gemma":0.00009717311,"threshold_uncertainty_score":0.006050229},"labels":[],"label_agreement":null},{"id":"W1984399020","doi":"10.1088/0004-637x/787/2/115","title":"AN EARLY LOOK OF COMET C/2013 A1 (SIDING SPRING): BREATHTAKER OR NIGHTMARE?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Meteoroid; Comet; Mars Exploration Program; Martian; Astrobiology; Atmosphere of Mars; Comet dust; Comet nucleus; Planet; Spacecraft; Spring (device); Physics; Comet tail; Astronomy; Environmental science; Interplanetary dust cloud; Solar System; Solar wind","score_opus":0.009115300356375767,"score_gpt":0.21816167589149477,"score_spread":0.209046375535119,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984399020","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9712605,0.0010921689,0.005810057,0.004373761,0.00034083065,0.000036640355,0.0020986858,0.00067345053,0.014313923],"genre_scores_gemma":[0.9955095,0.00014282904,0.0016726403,0.0002814616,0.00003763545,0.0000037282623,0.00095177785,0.000042371525,0.0013579606],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999398,0.000008764548,0.0000015414707,0.00001547856,0.0000134672055,0.000020982532],"domain_scores_gemma":[0.9998884,0.000018097755,0.000016698148,0.000009621513,0.000019478464,0.000047712343],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018695163,0.00030510506,0.00028004166,0.0002220411,0.00059965474,0.0006787119,0.00038552057,0.00094862806,0.0029555636],"category_scores_gemma":[0.00041084678,0.00011584663,0.00039885537,0.0001868146,0.00028406963,0.0007492561,0.0003507643,0.0006315618,0.00037771655],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018880218,0.00035687743,0.7347305,0.0004208385,0.0005200812,0.017542174,0.0029974112,0.049590085,0.06477482,0.017169934,0.06648562,0.043523666],"study_design_scores_gemma":[0.00017606652,0.0009489218,0.5939445,0.00017938115,0.00027294876,0.0046705385,0.005856877,0.29113922,0.018366527,0.013036394,0.07120858,0.00020014733],"about_ca_topic_score_codex":0.019540064,"about_ca_topic_score_gemma":0.035170645,"teacher_disagreement_score":0.019540064,"about_ca_system_score_codex":0.0007773219,"about_ca_system_score_gemma":0.00024231855,"threshold_uncertainty_score":0.03885269},"labels":[],"label_agreement":null},{"id":"W1984408118","doi":"10.1086/421513","title":"The Distance to the Large Magellanic Cloud Cluster Reticulum from the<i>K</i>‐Band Period‐Luminosity‐Metallicity Relation of RR Lyrae Stars","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"RR Lyrae variable; Physics; Metallicity; Astrophysics; Large Magellanic Cloud; Luminosity; Overtone; Cluster (spacecraft); Absolute magnitude; Distance modulus; Stars; Telescope; Astronomy; Galaxy; Globular cluster; Spectral line","score_opus":0.006711139327867312,"score_gpt":0.20868532816307278,"score_spread":0.20197418883520546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984408118","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989962,0.000046129513,0.00007351046,0.000010011738,8.7265784e-7,7.8960863e-7,0.0002208354,0.0000044918975,0.0006470914],"genre_scores_gemma":[0.9989906,0.00003818084,0.00016941101,0.0000028873817,0.000002748839,0.0000012299491,0.00062733603,0.000003223218,0.00016443744],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998889,0.00000762364,0.000005615276,0.00004302059,0.000028234399,0.000026550159],"domain_scores_gemma":[0.99938595,0.00010975184,0.00025220317,0.00006180787,0.00007798559,0.00011221244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001490633,0.00011308999,0.00011095705,0.0004854801,0.00048538132,0.0003628406,0.00025916862,0.00015856908,0.0007007725],"category_scores_gemma":[0.0008545508,0.00007387216,0.000084766405,0.00041619426,0.00020420898,0.00025046553,0.00051985437,0.00017568911,0.00033789146],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012566283,0.000011166558,0.9767054,0.00003323085,0.000024060215,0.00009025658,0.0005536027,0.0014344066,0.011704802,0.00065686635,0.00051890675,0.008141609],"study_design_scores_gemma":[0.000001722167,0.00001420651,0.9974111,0.00000277659,0.000005996588,0.00011171463,0.00007215487,0.0005019649,0.00057216326,0.000058200545,0.0012431993,0.0000047462527],"about_ca_topic_score_codex":0.013896562,"about_ca_topic_score_gemma":0.02544252,"teacher_disagreement_score":0.013896562,"about_ca_system_score_codex":0.00043531385,"about_ca_system_score_gemma":0.00026259487,"threshold_uncertainty_score":0.027631342},"labels":[],"label_agreement":null},{"id":"W1984518272","doi":"10.1088/0004-637x/783/1/29","title":"MOLECULAR OUTFLOWS DRIVEN BY LOW-MASS PROTOSTARS. I. CORRECTING FOR UNDERESTIMATES WHEN MEASURING OUTFLOW MASSES AND DYNAMICAL PROPERTIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Outflow; Protostar; Astrophysics; Physics; Opacity; Excitation; Excited state; Kinetic energy; Dissociation (chemistry); Luminosity; Molecular cloud; Atomic physics; Star formation; Stars; Chemistry","score_opus":0.015310736289670656,"score_gpt":0.2219965970432401,"score_spread":0.20668586075356943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984518272","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989849,0.0007293486,0.006048021,0.00016121287,0.000043656997,0.000021845564,0.00068937725,0.00018375742,0.0022737023],"genre_scores_gemma":[0.99638367,0.00015887611,0.002367816,0.000038084832,0.000026133517,0.000010729797,0.00062136457,0.000018838335,0.0003745298],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99963355,0.00007125699,0.000031045143,0.000111693415,0.00010158276,0.00005088609],"domain_scores_gemma":[0.99862885,0.00028979126,0.0006617187,0.00012626089,0.00019904452,0.00009426196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00113043,0.0002195871,0.00029496697,0.0009883107,0.0006156664,0.0008644019,0.00034501712,0.00037238785,0.00053592736],"category_scores_gemma":[0.003709575,0.00016701724,0.00017119323,0.0007624686,0.00028626615,0.0006960084,0.00073555,0.00029057168,0.00024896747],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026647028,0.0000371667,0.94076216,0.00006268882,0.00004939336,0.00010970316,0.00021515781,0.001570462,0.024143388,0.00051973836,0.0004728588,0.03179079],"study_design_scores_gemma":[0.000008668369,0.00004724127,0.9744425,0.000026424745,0.000038976294,0.00017019617,0.00018823841,0.013274817,0.009382683,0.000624317,0.0017847483,0.000011275901],"about_ca_topic_score_codex":0.004554998,"about_ca_topic_score_gemma":0.0067559974,"teacher_disagreement_score":0.004554998,"about_ca_system_score_codex":0.00045529875,"about_ca_system_score_gemma":0.00031993844,"threshold_uncertainty_score":0.009056926},"labels":[],"label_agreement":null},{"id":"W1984582474","doi":"10.1086/374266","title":"The Pulsar Wind Nebula in G11.2−0.3","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Nebula; Pulsar wind nebula; Supernova remnant; Emission nebula; Heliosphere; Synchrotron; Millisecond pulsar; Observatory","score_opus":0.010033933931219485,"score_gpt":0.3049310947052807,"score_spread":0.2948971607740612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984582474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996754,0.000056440724,0.000027976848,0.0000064651103,9.648252e-7,0.0000025221939,0.000032800086,0.0000034382767,0.00019395794],"genre_scores_gemma":[0.99903643,0.00006936726,0.00008973418,0.000026784044,0.000004998417,0.000004523443,0.00042511162,0.000004642285,0.00033846876],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995923,0.0000048879683,0.000002202035,0.0000111079535,0.0000052810124,0.000017418526],"domain_scores_gemma":[0.9998852,0.00001281675,0.00004034895,0.000008003067,0.000008766995,0.000044778775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010335166,0.00023129399,0.00022999608,0.0005494022,0.00035996202,0.00038382655,0.0001460148,0.00018609974,0.0007369175],"category_scores_gemma":[0.00020357774,0.00012740796,0.00013477978,0.000400642,0.00030562008,0.00013069576,0.0004097606,0.00019127768,0.00024911753],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090718817,0.00019096323,0.8962397,0.000036246176,0.00006948923,0.0030791538,0.0009953105,0.0005085357,0.08403967,0.00035186342,0.00038730196,0.013194634],"study_design_scores_gemma":[0.0000074627214,0.000102765254,0.9981186,0.000001861605,0.000006555675,0.00061024167,0.00010800119,0.00010788796,0.00038488212,0.000034405868,0.0005143203,0.0000028088014],"about_ca_topic_score_codex":0.0041638548,"about_ca_topic_score_gemma":0.0056306175,"teacher_disagreement_score":0.0041638548,"about_ca_system_score_codex":0.00021460639,"about_ca_system_score_gemma":0.00009466442,"threshold_uncertainty_score":0.008279264},"labels":[],"label_agreement":null},{"id":"W1984654140","doi":"10.1088/0004-637x/753/1/68","title":"THE TYPE II SUPERNOVA RATE IN<i>z</i>∼ 0.1 GALAXY CLUSTERS FROM THE MULTI-EPOCH NEARBY CLUSTER SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Supernova; Galaxy; Galaxy cluster; Astronomy; Cluster (spacecraft); Star formation; Redshift; Solar mass","score_opus":0.022858979133574316,"score_gpt":0.2532603682435839,"score_spread":0.23040138911000957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984654140","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961825,0.0002687328,0.00013974715,0.00003065736,0.0000045209085,0.000006872222,0.002177852,0.000035214256,0.0011539821],"genre_scores_gemma":[0.9956043,0.00015967332,0.00019279665,0.00002332663,0.000010539776,0.0000061735127,0.0035065075,0.000007960568,0.00048879255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999808,0.0000134369,0.000012731718,0.0000568449,0.00005427619,0.000054800465],"domain_scores_gemma":[0.9987907,0.00012219851,0.0005504828,0.00007224751,0.00019960127,0.00026493787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029322322,0.00027110524,0.00016916766,0.0023104786,0.00020732667,0.0004970322,0.00037665854,0.00020758163,0.0012728476],"category_scores_gemma":[0.0012801302,0.00013495416,0.00023855604,0.0009904249,0.00022162634,0.00028185666,0.00053328375,0.00021124793,0.0003535077],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000018340992,0.0000033346716,0.99651295,0.000010366476,0.000022482078,0.000022490207,0.000043958626,0.00016078184,0.0006131959,0.000059789138,0.00033853494,0.00219372],"study_design_scores_gemma":[8.488856e-7,0.000006583046,0.99935,0.0000017234229,0.000009149352,0.000046459238,0.000016514507,0.000105018706,0.00012400454,0.000012221394,0.0003259385,0.000001482745],"about_ca_topic_score_codex":0.05393749,"about_ca_topic_score_gemma":0.07942111,"teacher_disagreement_score":0.05393749,"about_ca_system_score_codex":0.0006693572,"about_ca_system_score_gemma":0.00025188565,"threshold_uncertainty_score":0.107247114},"labels":[],"label_agreement":null},{"id":"W1984683642","doi":"10.1086/592188","title":"H<scp>i</scp>Clouds in the Lower Halo. I. The Galactic All‐Sky Survey Pilot Region","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Halo; Galactic halo; Sky; Galaxy; Astronomy; Spiral galaxy; Galactic plane; Population; Star formation; RADIUS","score_opus":0.03923373098237433,"score_gpt":0.25536943227080194,"score_spread":0.21613570128842763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984683642","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99900585,0.00015888517,0.000032297063,0.00004242993,0.0000011987987,0.0000021915364,0.00021860926,0.0000052286173,0.0005332425],"genre_scores_gemma":[0.9994617,0.000050320537,0.000047647343,0.000016083977,0.0000042574547,9.965157e-7,0.00033896562,0.0000010110489,0.000078941106],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986255,0.000010145464,0.0000051262828,0.000019456149,0.00003150698,0.000071215436],"domain_scores_gemma":[0.99939775,0.00003940475,0.00025323525,0.000036989244,0.00007214259,0.0002004045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019313637,0.000097272045,0.00014362903,0.001087549,0.00051667716,0.0005810997,0.0002189864,0.00012512616,0.001017079],"category_scores_gemma":[0.00045645208,0.000102025915,0.000089323185,0.0012887586,0.0004051246,0.00027540195,0.0005305586,0.00013070971,0.00016262519],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000080198,0.00001187829,0.99003196,0.000017483982,0.000018783872,0.00010717942,0.00019967403,0.00009734194,0.00365807,0.00013486804,0.00038092522,0.0052615255],"study_design_scores_gemma":[0.0000025827003,0.000013162008,0.999111,0.000003948162,0.0000039662386,0.000053696254,0.0000702532,0.00008723022,0.00015497066,0.000030759827,0.0004674158,0.0000010980968],"about_ca_topic_score_codex":0.048764564,"about_ca_topic_score_gemma":0.07484352,"teacher_disagreement_score":0.048764564,"about_ca_system_score_codex":0.00046355507,"about_ca_system_score_gemma":0.00024517585,"threshold_uncertainty_score":0.09696144},"labels":[],"label_agreement":null},{"id":"W1984755196","doi":"10.1086/519377","title":"Strangers in the Night: Discovery of a Dwarf Spheroidal Galaxy on Its First Local Group Infall","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Local Group; Andromeda; Physics; Astrophysics; Dwarf galaxy; Galaxy; Astronomy; Andromeda Galaxy; Dwarf spheroidal galaxy; Dark galaxy; Orbit (dynamics); Milky Way; Interacting galaxy","score_opus":0.008951226756268494,"score_gpt":0.21620070379102765,"score_spread":0.20724947703475916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984755196","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99754167,0.00011740703,0.00011869597,0.00014238898,0.00001522264,0.0000031601253,0.00006870926,0.000016574002,0.001976126],"genre_scores_gemma":[0.9990701,0.00006260982,0.00014167209,0.0000683117,0.000023832183,9.720466e-7,0.00012897534,0.000004516358,0.00049910473],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994195,0.0000055523424,0.000002338822,0.000015060797,0.000011915229,0.000023120954],"domain_scores_gemma":[0.999736,0.000018869046,0.000036026922,0.000028403265,0.00001843481,0.000162288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015536352,0.00016330673,0.00022814574,0.00053828256,0.0012564571,0.0007672291,0.00021446077,0.0003699818,0.0012133429],"category_scores_gemma":[0.00032107913,0.0001491893,0.00017388536,0.00030204444,0.00057410315,0.00037232589,0.00094526104,0.0005733149,0.00030692323],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071691204,0.00014173317,0.9035474,0.00005010213,0.00004947056,0.018128067,0.0075459797,0.00011076269,0.04265576,0.0016636156,0.0027461667,0.022644028],"study_design_scores_gemma":[0.000015849067,0.0004121136,0.9699091,0.000018203935,0.00003512499,0.011670568,0.0030397463,0.00028630273,0.003547042,0.0006227562,0.010419705,0.00002349213],"about_ca_topic_score_codex":0.0033682014,"about_ca_topic_score_gemma":0.0057723676,"teacher_disagreement_score":0.0033682014,"about_ca_system_score_codex":0.00050008413,"about_ca_system_score_gemma":0.00014149782,"threshold_uncertainty_score":0.006697178},"labels":[],"label_agreement":null},{"id":"W1984805696","doi":"10.1088/0004-637x/761/2/168","title":"CAN DUST EMISSION BE USED TO ESTIMATE THE MASS OF THE INTERSTELLAR MEDIUM IN GALAXIES—A PILOT PROJECT WITH THE HERSCHEL REFERENCE SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Galaxy; Interstellar medium; Cosmic dust; Emissivity; Calibration; Line (geometry); Virgo Cluster","score_opus":0.03346589575516382,"score_gpt":0.2759115963648041,"score_spread":0.2424457006096403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984805696","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9592415,0.000951462,0.02972718,0.0006764729,0.00003936906,0.00024541054,0.00428162,0.0010111902,0.0038259868],"genre_scores_gemma":[0.94848883,0.0002325878,0.046794232,0.000090479356,0.000031714324,0.00010785035,0.0032433502,0.00012920449,0.00088172976],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9982827,0.0009467819,0.000039566457,0.0002987045,0.0002891575,0.00014312069],"domain_scores_gemma":[0.99652773,0.0008875763,0.0004388683,0.0011372939,0.0006587766,0.00034985042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0070486576,0.0005520149,0.0004949786,0.0012052808,0.0003500359,0.0011977341,0.0010445203,0.0006762082,0.00073654676],"category_scores_gemma":[0.005214261,0.00029284664,0.00044424357,0.0012567192,0.00042782142,0.0010624354,0.0007738346,0.00034047154,0.00051930314],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047244475,0.00026955828,0.885609,0.000083337865,0.00024763457,0.00010827158,0.00034645948,0.012508814,0.00992323,0.0011088924,0.0016069915,0.08771532],"study_design_scores_gemma":[0.0002210233,0.00044709846,0.93327636,0.00003535418,0.000109636116,0.00010911,0.00033424675,0.039509602,0.013517406,0.0010781569,0.011310642,0.00005140492],"about_ca_topic_score_codex":0.034277227,"about_ca_topic_score_gemma":0.026198903,"teacher_disagreement_score":0.034277227,"about_ca_system_score_codex":0.001061088,"about_ca_system_score_gemma":0.00059154397,"threshold_uncertainty_score":0.06815541},"labels":[],"label_agreement":null},{"id":"W1984821841","doi":"10.1088/0004-637x/756/1/61","title":"ON THE EXISTENCE OF “RADIO THERMALLY ACTIVE” GALACTIC SUPERNOVA REMNANTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Bremsstrahlung; Supernova; Flattening; Thermal; Thermal emission; Thermal radiation; Absorption (acoustics); Radiation; Polarization (electrochemistry)","score_opus":0.017475732764969946,"score_gpt":0.23422057926706974,"score_spread":0.2167448465020998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1984821841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9811695,0.0027928464,0.010154739,0.0001009991,0.00003894096,0.000010960049,0.00008545465,0.00011473306,0.0055316663],"genre_scores_gemma":[0.99785465,0.00056715606,0.0010774382,0.000046569017,0.000040609233,0.000002659907,0.00014336582,0.000015138686,0.00025243778],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997657,0.000051585328,0.00001680684,0.000073321724,0.000045106986,0.00004759429],"domain_scores_gemma":[0.99848217,0.0005423956,0.0005272674,0.00021232336,0.00013780194,0.00009796347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000941611,0.00047659694,0.0003503868,0.00068925245,0.0003899704,0.0009955686,0.00046460037,0.00048730613,0.0022289285],"category_scores_gemma":[0.0013593866,0.00021597414,0.0005722263,0.0004126378,0.0008089665,0.00055707956,0.00052187004,0.00030308552,0.0004340643],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011732209,0.000095418385,0.8530409,0.00061579805,0.000788273,0.008251286,0.00059108215,0.009492374,0.070611164,0.018289465,0.0005896622,0.03646125],"study_design_scores_gemma":[0.000076275806,0.0008656247,0.89240974,0.00024920588,0.0008992892,0.0114790555,0.0009802992,0.029522307,0.03662508,0.014738044,0.012061526,0.000093478324],"about_ca_topic_score_codex":0.00053712993,"about_ca_topic_score_gemma":0.00045594285,"teacher_disagreement_score":0.0022289285,"about_ca_system_score_codex":0.00019476503,"about_ca_system_score_gemma":0.00013327175,"threshold_uncertainty_score":0.0074564815},"labels":[],"label_agreement":null},{"id":"W1985060735","doi":"10.1088/0004-637x/708/1/584","title":"A COMPARISON OF X-RAY AND MID-INFRARED SELECTION OF OBSCURED ACTIVE GALACTIC NUCLEI","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Quest University Canada","funders":"","keywords":"Active galactic nucleus; Physics; Astrophysics; Infrared; Luminosity; Astronomy; Redshift; Luminous infrared galaxy; Galaxy","score_opus":0.009722666330439646,"score_gpt":0.24634016383487878,"score_spread":0.23661749750443914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985060735","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943749,0.00041588926,0.0006101714,0.000046641508,0.0000068587383,0.000008411568,0.00034624452,0.000026793365,0.0041641155],"genre_scores_gemma":[0.99618965,0.0002805853,0.0011371586,0.00006936189,0.000027797207,0.0000070804404,0.0014232415,0.000016984332,0.00084828294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99957865,0.0000831027,0.00003229731,0.00010003051,0.00012855274,0.000077344266],"domain_scores_gemma":[0.9982247,0.0006258631,0.00037025614,0.0002314975,0.00035334504,0.00019446267],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089559983,0.00014302687,0.00018801942,0.0015278602,0.000203274,0.0007686012,0.00038954127,0.00020317285,0.0014791328],"category_scores_gemma":[0.0024548068,0.000097175995,0.00017075731,0.00058752677,0.0001930721,0.00051243027,0.00055150216,0.00012667252,0.0004790759],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009957716,0.000083532985,0.93167365,0.00007020156,0.00009236829,0.00012625237,0.00027927436,0.0008349153,0.018696968,0.0006516543,0.0006616911,0.045833666],"study_design_scores_gemma":[0.000018742552,0.00013247026,0.9914784,0.000019252657,0.00003862899,0.0002301945,0.00021328346,0.0022632643,0.0038763725,0.00018983561,0.0015294987,0.000010063653],"about_ca_topic_score_codex":0.002577787,"about_ca_topic_score_gemma":0.0073193996,"teacher_disagreement_score":0.002577787,"about_ca_system_score_codex":0.00024214372,"about_ca_system_score_gemma":0.00014755032,"threshold_uncertainty_score":0.005125582},"labels":[],"label_agreement":null},{"id":"W1985089268","doi":"10.1088/0004-637x/694/2/1161","title":"STAR FORMATION AT VERY LOW METALLICITY. V. THE GREATER IMPORTANCE OF INITIAL CONDITIONS COMPARED TO METALLICITY THRESHOLDS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Metallicity; Physics; Astrophysics; Stars; Halo; Star formation; Turbulence; Ionization; Initial mass function; Galaxy; Mechanics; Ion","score_opus":0.015255379391846714,"score_gpt":0.2548308875397327,"score_spread":0.239575508147886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985089268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99202406,0.00018085274,0.0032951112,0.00023908402,0.000009809298,0.000018432453,0.00010692448,0.00011246165,0.00401323],"genre_scores_gemma":[0.9991254,0.000050605347,0.00042844354,0.00003165869,0.0000033222645,0.0000052548094,0.00004083851,0.000010073076,0.00030447415],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991465,0.000012232522,0.000004143356,0.000017942324,0.00001596347,0.000035034547],"domain_scores_gemma":[0.99957746,0.00011972458,0.000080703416,0.000034664856,0.00003433629,0.00015320399],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018257539,0.0002141363,0.00033239662,0.00023597018,0.00044128805,0.0012941011,0.00033434457,0.00059382105,0.0024482359],"category_scores_gemma":[0.0014657325,0.00020060517,0.00031764744,0.0001525382,0.00080059073,0.00060610025,0.00074337405,0.00053795584,0.00030735103],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007891478,0.00025591432,0.31226164,0.0005578281,0.00023818454,0.0022960585,0.0013506034,0.3855664,0.20501867,0.06628915,0.0026269103,0.022749426],"study_design_scores_gemma":[0.00028312023,0.0008269248,0.35199988,0.00016883381,0.00015311064,0.0011574291,0.0014279397,0.5016714,0.042603962,0.09311221,0.0064648315,0.00013034446],"about_ca_topic_score_codex":0.0029868234,"about_ca_topic_score_gemma":0.0019377539,"teacher_disagreement_score":0.0029868234,"about_ca_system_score_codex":0.00087705033,"about_ca_system_score_gemma":0.0003670158,"threshold_uncertainty_score":0.008190155},"labels":[],"label_agreement":null},{"id":"W1985243060","doi":"10.1088/0004-637x/799/1/29","title":"THE BOLOCAM GALACTIC PLANE SURVEY. XII. DISTANCE CATALOG EXPANSION USING KINEMATIC ISOLATION OF DENSE MOLECULAR CLOUD STRUCTURES WITH<sup>13</sup>CO(1-0)","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galactic plane; Molecular cloud; Kinematics; Galactic Center; Astrometry; Trigonometric functions; Galaxy","score_opus":0.016088184487228915,"score_gpt":0.2537032211773344,"score_spread":0.23761503669010547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985243060","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2773425,0.007610693,0.01946923,0.0014698234,0.0003294217,0.0008164369,0.6078269,0.004437392,0.08069761],"genre_scores_gemma":[0.24143186,0.0037512719,0.063670926,0.0004951691,0.00030259942,0.00050334306,0.67439115,0.0005950677,0.014858678],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996798,0.00002971092,0.000023060287,0.00007250075,0.00015925626,0.000035684636],"domain_scores_gemma":[0.99908745,0.000043474407,0.0002763624,0.00020058584,0.0002758829,0.00011632467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005625823,0.00041257998,0.00019617703,0.0039316914,0.00021432992,0.0009798155,0.0006575778,0.0002798172,0.0041552237],"category_scores_gemma":[0.0013869229,0.00021039361,0.0001923995,0.004832216,0.0001607477,0.0004990905,0.001009083,0.00040878734,0.0053207106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024704644,0.00004367683,0.5185804,0.00036862944,0.00011359667,0.00022764369,0.0002821063,0.0017166209,0.0070401756,0.0030657533,0.18109368,0.28722066],"study_design_scores_gemma":[0.00003528788,0.000026378435,0.79390633,0.00008807087,0.00003016301,0.00015057418,0.00010359407,0.0013087508,0.0015531193,0.0005142714,0.20227309,0.0000103573075],"about_ca_topic_score_codex":0.056711126,"about_ca_topic_score_gemma":0.07819156,"teacher_disagreement_score":0.056711126,"about_ca_system_score_codex":0.0011553735,"about_ca_system_score_gemma":0.00079804147,"threshold_uncertainty_score":0.11276209},"labels":[],"label_agreement":null},{"id":"W1985296727","doi":"10.1088/0004-637x/727/2/114","title":"THE BALLOON-BORNE LARGE APERTURE SUBMILLIMETER TELESCOPE (BLAST) 2005: A 10 deg<sup>2</sup>SURVEY OF STAR FORMATION IN CYGNUS X","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of British Columbia; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Star formation; Astronomy; Spectral energy distribution; Luminosity; Stars; Protostar; Context (archaeology); Galaxy","score_opus":0.017659432245535445,"score_gpt":0.22773481563073902,"score_spread":0.21007538338520357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985296727","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906855,0.00046766747,0.0016275649,0.00020258415,0.000011391429,0.000023883438,0.0039657303,0.00021050115,0.0028052581],"genre_scores_gemma":[0.97826195,0.00034615045,0.009174319,0.00019759829,0.00007256151,0.000035469777,0.010296708,0.0000633377,0.0015519854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998228,0.00003335459,0.000009627628,0.000044208897,0.00005126957,0.00003875907],"domain_scores_gemma":[0.9993468,0.000057589292,0.00026868607,0.00008652221,0.00006755414,0.00017290922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050692796,0.00034209804,0.00025999724,0.0014773866,0.00030534572,0.00047298762,0.00043471257,0.00042432806,0.00094951695],"category_scores_gemma":[0.00058462424,0.00020506105,0.00017885819,0.001357753,0.0002549996,0.00036648576,0.0007606735,0.00027852657,0.0006320824],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002464997,0.00003888745,0.94372475,0.000059124737,0.00010520461,0.000379041,0.0003761946,0.0012719352,0.028518196,0.0006383602,0.00312702,0.021514691],"study_design_scores_gemma":[0.0000071350655,0.000034481658,0.9951866,0.0000066700554,0.000014572743,0.00021755368,0.000055538356,0.00068361673,0.0011464296,0.000131575,0.0025104345,0.000005431039],"about_ca_topic_score_codex":0.007191622,"about_ca_topic_score_gemma":0.023690546,"teacher_disagreement_score":0.007191622,"about_ca_system_score_codex":0.0005175555,"about_ca_system_score_gemma":0.00026971253,"threshold_uncertainty_score":0.014299512},"labels":[],"label_agreement":null},{"id":"W1985304183","doi":"10.1086/374589","title":"The Pleiades Reflection Nebula. I. Ultraviolet, Optical, and Far‐Infrared Imaging Photometry","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Nebula; Reflection nebula; Astrophysics; Photometry (optics); Astronomy; Stars; Pleiades; Ultraviolet; Extinction (optical mineralogy); Optics","score_opus":0.009559579236131453,"score_gpt":0.2430790513198758,"score_spread":0.23351947208374435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985304183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9298425,0.0028974018,0.007087119,0.00032075294,0.00004644423,0.0000647046,0.007399488,0.0015642546,0.05077745],"genre_scores_gemma":[0.96593994,0.0009737428,0.016353197,0.000184329,0.00005961803,0.000025494146,0.008637415,0.0001669873,0.0076592043],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998859,0.000008408146,0.0000037164468,0.00003518683,0.00005085983,0.00001589491],"domain_scores_gemma":[0.9999089,0.0000065661625,0.000028979752,0.000020053023,0.000017627754,0.000017834353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001536689,0.00033057822,0.0001658059,0.00067011605,0.00030571362,0.00049981393,0.00022649202,0.00017388137,0.0039604562],"category_scores_gemma":[0.00014754469,0.00022215015,0.00022622934,0.00040853626,0.00018147174,0.0003618916,0.00036987974,0.0003194901,0.0014904751],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050786394,0.00016908799,0.5429174,0.0005414452,0.00014388599,0.0008799786,0.0012774378,0.0015898569,0.26859728,0.0025496231,0.017239165,0.16358693],"study_design_scores_gemma":[0.00001877859,0.000097426455,0.9746114,0.00002351332,0.000017571809,0.0013484409,0.000112253685,0.0004754648,0.0027873048,0.00020517418,0.02029528,0.000007386816],"about_ca_topic_score_codex":0.0029829694,"about_ca_topic_score_gemma":0.0056638224,"teacher_disagreement_score":0.0039604562,"about_ca_system_score_codex":0.00018264417,"about_ca_system_score_gemma":0.0001451299,"threshold_uncertainty_score":0.01324904},"labels":[],"label_agreement":null},{"id":"W1985342635","doi":"10.1088/0004-637x/708/2/1002","title":"THE INITIAL CONDITIONS OF CLUSTERED STAR FORMATION. II. N<sub>2</sub>H<sup>+</sup>OBSERVATIONS OF THE OPHIUCHUS B CORE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Astrophysics; Physics; Molecular cloud; Protostar; Line (geometry); Star formation; Astronomy; Stars; Geometry","score_opus":0.027552661233123943,"score_gpt":0.2627086683030085,"score_spread":0.23515600706988454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985342635","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962627,0.00023448425,0.0005208739,0.000038921775,0.000004154171,0.000023130937,0.00033446235,0.000020745576,0.0025604225],"genre_scores_gemma":[0.9987748,0.000055982862,0.00038233981,0.0000147133915,0.0000041951726,0.00000886036,0.00036781552,0.000003231111,0.00038816655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999138,0.0000056968765,0.000005272228,0.000023755238,0.000022584765,0.000029006269],"domain_scores_gemma":[0.9997205,0.00002196846,0.00007199026,0.000023481154,0.00005264193,0.00010939999],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011120819,0.00018146861,0.0001717028,0.00029457913,0.00055263116,0.00045948723,0.00027667286,0.00031251332,0.001373675],"category_scores_gemma":[0.0006015334,0.00016552093,0.00010631598,0.0001989123,0.00024146706,0.00025267265,0.0005073492,0.00025170846,0.00050916255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004662935,0.00008453262,0.77810013,0.00016773798,0.000055776396,0.0012229696,0.0007219314,0.0042448095,0.19976781,0.0027262897,0.0013677826,0.011073923],"study_design_scores_gemma":[0.000020312304,0.00012428255,0.98005474,0.000014796893,0.000012685104,0.0005863578,0.000526733,0.0026304321,0.012573318,0.00090083195,0.0025438687,0.000011611468],"about_ca_topic_score_codex":0.011058676,"about_ca_topic_score_gemma":0.015515807,"teacher_disagreement_score":0.011058676,"about_ca_system_score_codex":0.00091870636,"about_ca_system_score_gemma":0.00040868894,"threshold_uncertainty_score":0.02198863},"labels":[],"label_agreement":null},{"id":"W1985445679","doi":"10.1088/0004-637x/722/1/88","title":"X-RAY VARIABILITY AND EVIDENCE FOR PULSATIONS FROM THE UNIQUE RADIO PULSAR/X-RAY BINARY TRANSITION OBJECT FIRST J102347.6+003841","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Office of Experimental Program to Stimulate Competitive Research; Fonds Québécois de la Recherche sur la Nature et les Technologies; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canadian Institute for Advanced Research; National Aeronautics and Space Administration","keywords":"Millisecond pulsar; Pulsar; Binary pulsar; Pulsar planet; Orbital period; X-ray pulsar; Binary number; Orbital elements; Millisecond; Binary star","score_opus":0.020810835410447908,"score_gpt":0.25725112307319437,"score_spread":0.23644028766274647,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985445679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99924386,0.00005810865,0.000026340966,0.000011510677,0.000002095778,0.000005055059,0.00007358046,0.000004952777,0.00057446625],"genre_scores_gemma":[0.9987243,0.00005385899,0.00023065254,0.00002291641,0.000015942733,0.000008336033,0.0006182143,0.0000038438034,0.00032198278],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997701,0.000016265587,0.000016185202,0.000061228704,0.00007035085,0.00006583769],"domain_scores_gemma":[0.99954385,0.00003983265,0.00022181979,0.00003906453,0.000049448212,0.000105922685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026012643,0.0003047251,0.00037922527,0.00093105296,0.0007303474,0.0006177106,0.00036395632,0.00045798798,0.0011757173],"category_scores_gemma":[0.00044106558,0.0002644445,0.00012005586,0.00093040825,0.00036166987,0.0002652427,0.0006281419,0.0003068153,0.00029444828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036553113,0.00024033166,0.8499135,0.000091336435,0.000062790474,0.0025674133,0.00071801257,0.00031165956,0.12624897,0.00034060964,0.0006116325,0.018528176],"study_design_scores_gemma":[0.000018791612,0.0001680885,0.99510276,0.000004570392,0.00001382878,0.002136105,0.00009904302,0.00021570851,0.0010495237,0.0000619926,0.0011237921,0.0000058192163],"about_ca_topic_score_codex":0.0015740583,"about_ca_topic_score_gemma":0.0034024527,"teacher_disagreement_score":0.0015740583,"about_ca_system_score_codex":0.00028047292,"about_ca_system_score_gemma":0.00012968312,"threshold_uncertainty_score":0.0039331913},"labels":[],"label_agreement":null},{"id":"W1985508886","doi":"10.1086/381796","title":"The Submillimeter Properties of Extremely Red Objects in the Canada‐UK Deep Submillimeter Survey Fields","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Flux (metallurgy); Submillimeter Array; Astrophysics; Astronomy; Far infrared; Infrared; Population; Galaxy; Materials science; Star formation","score_opus":0.02055214936767486,"score_gpt":0.2049973199201846,"score_spread":0.18444517055250975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985508886","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936625,0.00026011482,0.00016096447,0.000055679047,0.0000025708607,0.0000065349336,0.002264799,0.000016817217,0.0035699152],"genre_scores_gemma":[0.99576724,0.00014100726,0.00021529151,0.000044600863,0.0000043537757,0.000005897539,0.0024556846,0.0000072383887,0.0013586835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996909,0.000011985875,0.000010579576,0.000045491543,0.00008578799,0.00015526246],"domain_scores_gemma":[0.9986638,0.00014727023,0.00037141054,0.00010417449,0.0003912156,0.00032219582],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027786638,0.00025585564,0.00019798455,0.0027083291,0.00081662444,0.0007879636,0.00041964327,0.0001834451,0.0015565658],"category_scores_gemma":[0.0011017433,0.00021556103,0.00014709265,0.0025026512,0.0004921434,0.0003007465,0.0007508154,0.00022215227,0.00031967228],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008047641,0.000008411514,0.9820839,0.00002133373,0.000019233317,0.00007502372,0.0007420336,0.00024342992,0.0036438727,0.00039875496,0.0012219193,0.011461735],"study_design_scores_gemma":[7.329951e-7,0.0000016460808,0.99922264,0.0000033142933,0.000002544394,0.0000146119155,0.000091076945,0.000048444046,0.00011777547,0.00001238459,0.0004827254,0.000001991792],"about_ca_topic_score_codex":0.79878134,"about_ca_topic_score_gemma":0.88890105,"teacher_disagreement_score":0.20121866,"about_ca_system_score_codex":0.0033817482,"about_ca_system_score_gemma":0.00092988356,"threshold_uncertainty_score":0.40480733},"labels":[],"label_agreement":null},{"id":"W1985527581","doi":"10.1088/0004-637x/732/1/44","title":"THE ATACAMA COSMOLOGY TELESCOPE: COSMOLOGY FROM GALAXY CLUSTERS DETECTED VIA THE SUNYAEV-ZEL'DOVICH EFFECT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":174,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Physics; CMB cold spot; Astrophysics; Galaxy cluster; South Pole Telescope; Cosmology; Sunyaev–Zel'dovich effect; Cosmic microwave background; Planck; Cluster (spacecraft); Observational cosmology; Galaxy; Dark energy","score_opus":0.007527883227442703,"score_gpt":0.20546814924075016,"score_spread":0.19794026601330744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985527581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8437426,0.0019200649,0.009668713,0.00164819,0.00026587048,0.00019401217,0.089550376,0.0018740081,0.051136155],"genre_scores_gemma":[0.93166447,0.00051128294,0.0127668325,0.000249849,0.00017104988,0.00013256693,0.046614747,0.00038576731,0.007503559],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999767,0.00003311742,0.000007294864,0.00006242066,0.00007978616,0.000050453556],"domain_scores_gemma":[0.9991007,0.00009899896,0.00018373395,0.00019313896,0.00015199198,0.00027148475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066784257,0.00019911383,0.00026416176,0.0023636848,0.000796185,0.0009643648,0.0004196253,0.0003841203,0.0043390044],"category_scores_gemma":[0.0015206583,0.00021979529,0.00032823862,0.002525374,0.00028111326,0.00064752786,0.0011611887,0.00054152205,0.0012570202],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039250593,0.00011741728,0.80680263,0.00022661067,0.0003574082,0.00046914042,0.0014151381,0.0017927788,0.0131573,0.0072458764,0.09078972,0.077233456],"study_design_scores_gemma":[0.00003405384,0.00001349578,0.9749638,0.000016173019,0.000025290185,0.00010686539,0.00017241632,0.0012066828,0.00057097885,0.00073861936,0.022135908,0.00001576183],"about_ca_topic_score_codex":0.030664679,"about_ca_topic_score_gemma":0.07031056,"teacher_disagreement_score":0.030664679,"about_ca_system_score_codex":0.00050430564,"about_ca_system_score_gemma":0.00075902796,"threshold_uncertainty_score":0.060972393},"labels":[],"label_agreement":null},{"id":"W1985533935","doi":"10.1086/504252","title":"An Upper Limit on the Albedo of HD 209458b: Direct Imaging Photometry with the<i>MOST</i>Satellite","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":176,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Saint Mary's University; St. Mary's University; University of British Columbia","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Exoplanet; Geometric albedo; Planet; Brightness; Astronomy; Light curve; Stars","score_opus":0.005991223867787994,"score_gpt":0.2070866552972636,"score_spread":0.2010954314294756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985533935","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9709937,0.0006847986,0.004416544,0.00017539648,0.000039313592,0.000029829502,0.005391276,0.00042571034,0.017843349],"genre_scores_gemma":[0.9888348,0.00015014419,0.0042772223,0.00012099832,0.00005609424,0.000036900678,0.0058605373,0.000063161686,0.0006001473],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997534,0.000024314215,0.00001520593,0.00007586061,0.00006825987,0.000062867206],"domain_scores_gemma":[0.9996345,0.000059621823,0.00010272707,0.00006386479,0.000072521456,0.00006666866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024744746,0.00040222958,0.000275048,0.0010195047,0.00048261945,0.00058841915,0.00028910712,0.00041559836,0.0024969522],"category_scores_gemma":[0.00050227804,0.00018657574,0.00023245333,0.00051338243,0.0002039564,0.00034097178,0.00065512664,0.0003562633,0.00063826126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000660482,0.00016615358,0.66936123,0.0002892764,0.000117453455,0.00026110825,0.00047370818,0.0019310223,0.2729781,0.0017660158,0.0080120135,0.043983262],"study_design_scores_gemma":[0.000019644849,0.00008926045,0.9678457,0.0000336301,0.000034734745,0.00030357714,0.000075767006,0.0013045421,0.020621572,0.00032192518,0.009336159,0.000013467063],"about_ca_topic_score_codex":0.004154829,"about_ca_topic_score_gemma":0.006962793,"teacher_disagreement_score":0.004154829,"about_ca_system_score_codex":0.00048883096,"about_ca_system_score_gemma":0.00014634307,"threshold_uncertainty_score":0.008353174},"labels":[],"label_agreement":null},{"id":"W1985554632","doi":"10.1086/430099","title":"Ultra–High‐Energy Cosmic Rays from Hypothetical Quark Novae","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Cosmic ray; Pulsar; Neutron star; Astronomy; Supernova; Ultra-high-energy cosmic ray; Vela; Pierre Auger Observatory","score_opus":0.006845969994667433,"score_gpt":0.20144763892345477,"score_spread":0.19460166892878733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985554632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9698197,0.00030684134,0.009703331,0.0002764277,0.000033970766,0.000031254476,0.0002961035,0.0001292695,0.019402958],"genre_scores_gemma":[0.99730814,0.0001223765,0.0011623938,0.0000383175,0.0000119079195,0.000009993582,0.00019679939,0.000016182432,0.0011338786],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998903,0.000034731933,0.000003505052,0.000017370432,0.000019363355,0.000034827328],"domain_scores_gemma":[0.9997249,0.00008968981,0.000059673977,0.000024521818,0.00002499991,0.00007606281],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003372893,0.0005526551,0.0003900922,0.00040311343,0.00063802954,0.0011151221,0.00057744276,0.0007949409,0.0032395844],"category_scores_gemma":[0.0007880717,0.00026225133,0.00061031483,0.00043344783,0.00054573885,0.00065290893,0.00088387716,0.000407185,0.0003235611],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093870546,0.000433687,0.23080271,0.00030453457,0.0002871416,0.008616799,0.00052806217,0.5392546,0.019464105,0.17953303,0.0028657338,0.016970847],"study_design_scores_gemma":[0.00019811456,0.00032622227,0.08198717,0.000058735375,0.00009126363,0.0012871573,0.0003895432,0.8406158,0.003923587,0.06700068,0.0040478013,0.00007387717],"about_ca_topic_score_codex":0.0035550876,"about_ca_topic_score_gemma":0.002761487,"teacher_disagreement_score":0.0035550876,"about_ca_system_score_codex":0.0008134243,"about_ca_system_score_gemma":0.00023556936,"threshold_uncertainty_score":0.010837436},"labels":[],"label_agreement":null},{"id":"W1985612581","doi":"10.1088/0004-637x/757/1/76","title":"DO R CORONAE BOREALIS STARS FORM FROM DOUBLE WHITE DWARF MERGERS?","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"White dwarf; Stars; Mass ratio; Physics; Astrophysics; Degenerate energy levels; Binary number; Mathematics","score_opus":0.01693293976603784,"score_gpt":0.2389603999686268,"score_spread":0.22202746020258896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985612581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99744534,0.0002653616,0.00026440772,0.00014504703,0.0000069458156,0.000011665625,0.000034191376,0.000020818052,0.0018062845],"genre_scores_gemma":[0.9996773,0.000072438495,0.00008882405,0.00002424087,0.0000067353703,0.0000017388284,0.0000390277,0.000002225612,0.00008730364],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997886,0.000041835872,0.000012218714,0.000050704413,0.00004123317,0.00006536493],"domain_scores_gemma":[0.9992705,0.00011678231,0.00034030998,0.00006190685,0.000028711875,0.00018173533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057949155,0.00031675355,0.00046416902,0.0005103017,0.000507056,0.0012504107,0.00048571223,0.0010669824,0.0011900471],"category_scores_gemma":[0.0019205677,0.0003198058,0.00044864454,0.00032538245,0.0006547874,0.00092752196,0.0007501295,0.00028076454,0.0003125896],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007615688,0.00027055,0.9416438,0.000128649,0.0002982343,0.0045435294,0.0010734649,0.008044954,0.01673839,0.004755263,0.00091918284,0.020822406],"study_design_scores_gemma":[0.00040353392,0.0007588642,0.89181405,0.000057849305,0.0002533781,0.008502914,0.003392587,0.069040194,0.005819454,0.011148269,0.008738719,0.00007034217],"about_ca_topic_score_codex":0.0020212317,"about_ca_topic_score_gemma":0.0025596446,"teacher_disagreement_score":0.0020212317,"about_ca_system_score_codex":0.00041448383,"about_ca_system_score_gemma":0.00024915033,"threshold_uncertainty_score":0.0040189624},"labels":[],"label_agreement":null},{"id":"W1985647485","doi":"10.1086/423737","title":"An Extinction Threshold for Protostellar Cores in Ophiuchus","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":198,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Physics; James Clerk Maxwell Telescope; Astrophysics; Extinction (optical mineralogy); Sky; Bolometer; Molecular cloud; Astronomy; Telescope; Star formation; Galaxy; Stars; Optics; Detector","score_opus":0.01509101076565468,"score_gpt":0.2679339447073054,"score_spread":0.25284293394165075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985647485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994485,0.000030430156,0.0001532032,0.0000068482836,4.7789104e-7,0.000003075568,0.00003483648,0.0000098073015,0.00031289476],"genre_scores_gemma":[0.9996966,0.0000108847835,0.00017164431,0.0000050369026,8.3244413e-7,0.000002073237,0.0000746616,0.0000021161616,0.00003611301],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998965,0.000011001014,0.000008871589,0.000023047742,0.000026689353,0.000033835913],"domain_scores_gemma":[0.9994466,0.000115877454,0.00018908655,0.00002396019,0.000080922655,0.00014361987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002636319,0.00012219591,0.000149586,0.00065314636,0.00035222885,0.00046681915,0.00026557822,0.00018645835,0.0007504759],"category_scores_gemma":[0.0013203941,0.00013409408,0.00011109245,0.00024948787,0.00021186071,0.00029914227,0.0003791125,0.00013811848,0.00010032637],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008665298,0.000034478926,0.9669238,0.00001546663,0.000012804666,0.00020328032,0.00018598416,0.0004873059,0.028693756,0.00016378988,0.000069363916,0.0031233474],"study_design_scores_gemma":[0.0000048346183,0.000028191786,0.996253,0.0000051012053,0.000005265093,0.00014621041,0.00010032166,0.0011527719,0.002076975,0.00011728957,0.00010760449,0.0000024753078],"about_ca_topic_score_codex":0.007826968,"about_ca_topic_score_gemma":0.011513406,"teacher_disagreement_score":0.007826968,"about_ca_system_score_codex":0.00046236286,"about_ca_system_score_gemma":0.00019601213,"threshold_uncertainty_score":0.015562773},"labels":[],"label_agreement":null},{"id":"W1985697011","doi":"10.1088/0004-637x/698/1/808","title":"POLYYNES AND INTERSTELLAR CARBON NANOPARTICLES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Carbon fibers; Molecule; Physics; Carbon Nanoparticles; Interstellar medium; Infrared; Absorption (acoustics); Astrochemistry; Carbon chain; Nanoparticle; Spectral line; Infrared spectroscopy; Absorption spectroscopy; Photochemistry; Astrophysics; Materials science; Chemistry; Astronomy; Organic chemistry; Composite number; Optics; Galaxy; Composite material","score_opus":0.007337519820359692,"score_gpt":0.22176629639355877,"score_spread":0.2144287765731991,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985697011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879439,0.0023002385,0.0023330532,0.00008172442,0.000030215295,0.000011155728,0.000049641127,0.000016993268,0.0072330707],"genre_scores_gemma":[0.99414045,0.0006292151,0.0010531638,0.000051515344,0.000006833437,0.0000070092638,0.00006699314,0.0000049115397,0.0040397705],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993813,0.000007691011,0.0000024847104,0.000022372462,0.00001828657,0.000011119124],"domain_scores_gemma":[0.9999291,0.000019323816,0.000025689114,0.0000063544826,0.000008631175,0.0000108923205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005735099,0.00016777987,0.00004353015,0.00012108831,0.00008850592,0.00019361114,0.000120444456,0.0002760713,0.0011056588],"category_scores_gemma":[0.00010648216,0.00007037772,0.000065788125,0.00006727092,0.00013410674,0.00020666135,0.00017730336,0.00018281928,0.00021627746],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051172265,0.000016233713,0.000741236,0.000047642876,0.000008557519,0.0002546704,0.000025606478,0.00033392542,0.99402606,0.0009763427,0.000075599,0.003443012],"study_design_scores_gemma":[0.000008806935,0.00020813277,0.006513367,0.000011071387,0.000008250641,0.00046111713,0.00003678975,0.0012403287,0.985537,0.00038661534,0.005583585,0.0000049583105],"about_ca_topic_score_codex":0.00035782685,"about_ca_topic_score_gemma":0.00065886474,"teacher_disagreement_score":0.0011056588,"about_ca_system_score_codex":0.00014889924,"about_ca_system_score_gemma":0.00005669201,"threshold_uncertainty_score":0.0036988258},"labels":[],"label_agreement":null},{"id":"W1985768552","doi":"10.1088/0004-637x/777/2/148","title":"SUPERNOVA REMNANT KES 17: AN EFFICIENT COSMIC RAY ACCELERATOR INSIDE A MOLECULAR CLOUD","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Cosmic ray; Physics; Supernova; Astrophysics; Supernova remnant; Molecular cloud; Astronomy; Near-Earth supernova; Acceleration","score_opus":0.009122346331430244,"score_gpt":0.22039706237368567,"score_spread":0.21127471604225542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985768552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99868256,0.00012600869,0.00023766447,0.000009361924,0.0000035660855,0.000003980233,0.000043334654,0.000027181028,0.0008663684],"genre_scores_gemma":[0.9989767,0.00005744052,0.0005080249,0.0000060277766,0.000004853146,0.0000011442917,0.00013975715,0.000006737534,0.00029929352],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994564,0.0000049432647,0.000003418618,0.000011199824,0.00001483519,0.000019961979],"domain_scores_gemma":[0.99976903,0.000015802641,0.00008269773,0.000031465992,0.000023712148,0.00007728238],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016982008,0.0002002163,0.0002782468,0.00032885754,0.00026278218,0.00059483445,0.00024222893,0.00013209651,0.0006816432],"category_scores_gemma":[0.00019378863,0.00011413501,0.00016839437,0.00022727033,0.00029216727,0.00021657647,0.0003987816,0.00016176268,0.0002665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013428438,0.00019881206,0.57267493,0.0001481125,0.00027594267,0.011242685,0.00029010457,0.0044659083,0.38062185,0.0054659033,0.0009384695,0.022334374],"study_design_scores_gemma":[0.00016543362,0.0013904368,0.8407276,0.00004447662,0.00029575746,0.017727464,0.000713225,0.019123571,0.098125905,0.0017552259,0.019879125,0.000051751424],"about_ca_topic_score_codex":0.0014160555,"about_ca_topic_score_gemma":0.002113372,"teacher_disagreement_score":0.0014160555,"about_ca_system_score_codex":0.0002390843,"about_ca_system_score_gemma":0.00022192596,"threshold_uncertainty_score":0.0028155446},"labels":[],"label_agreement":null},{"id":"W1985809928","doi":"10.1086/345493","title":"Radio Emission from Magnetars","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Narrowband; Bursting; Radio spectrum; Solar flare; Dissipation; Astronomy; Radio wave; Radio frequency; Neutron star; Optics; Telecommunications; Computer science","score_opus":0.014575347005723799,"score_gpt":0.2810709477352461,"score_spread":0.2664956007295223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985809928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97736174,0.004408733,0.005888685,0.00018687164,0.000039146562,0.000016806614,0.0003043202,0.00015105167,0.011642651],"genre_scores_gemma":[0.9947626,0.0015784928,0.0011859242,0.00012527002,0.00012874839,0.000014958488,0.00048436783,0.000029636001,0.0016899554],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993896,0.000008204263,0.0000025665308,0.00002000736,0.000008173252,0.000022010865],"domain_scores_gemma":[0.999881,0.0000390805,0.000037744772,0.000013985357,0.000011930239,0.000016200092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012759677,0.00034692456,0.00018687484,0.0004746771,0.00028394102,0.00051963987,0.00026120103,0.0004177118,0.0018184452],"category_scores_gemma":[0.00025026596,0.00009968182,0.00021081288,0.0003244009,0.0001746149,0.00032412514,0.00036264988,0.0001996052,0.00056772435],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010486962,0.00009965853,0.11363162,0.0005794067,0.00015981118,0.004626972,0.0006959116,0.0027828368,0.81099373,0.009719846,0.0027935926,0.052867893],"study_design_scores_gemma":[0.00016802673,0.001543812,0.762911,0.0001331223,0.00037197905,0.018763477,0.0006029415,0.008022808,0.16238381,0.008039342,0.036955215,0.00010446707],"about_ca_topic_score_codex":0.0001253729,"about_ca_topic_score_gemma":0.0001294858,"teacher_disagreement_score":0.0018184452,"about_ca_system_score_codex":0.00013332361,"about_ca_system_score_gemma":0.000021794078,"threshold_uncertainty_score":0.0060833097},"labels":[],"label_agreement":null},{"id":"W1985930112","doi":"10.1088/0004-637x/704/2/1036","title":"THE CARNEGIE SUPERNOVA PROJECT: FIRST NEAR-INFRARED HUBBLE DIAGRAM TO<i>z</i>∼ 0.7","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Dark energy; Redshift; Baryon acoustic oscillations; Luminosity distance; Astrophysics; Supernova; Cosmology; Luminosity; Hubble's law; Photometric redshift; Baryon; Universe; Observational cosmology; Astronomy; Galaxy","score_opus":0.011652183600266066,"score_gpt":0.24350360074266553,"score_spread":0.23185141714239946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1985930112","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.45042393,0.0072646737,0.16504623,0.0042126565,0.0008358075,0.000612343,0.08051879,0.007134816,0.28395063],"genre_scores_gemma":[0.84953296,0.0016214291,0.096653484,0.0005967769,0.00025972235,0.0004702583,0.036390293,0.00085392845,0.013621158],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9996252,0.00007726515,0.000011289667,0.000100952435,0.00012440927,0.000060835762],"domain_scores_gemma":[0.99828535,0.0002053919,0.00023034391,0.0001728884,0.00069114415,0.00041475828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013792719,0.00053360965,0.0002626354,0.0031632818,0.00067258807,0.0010111973,0.0004426054,0.0003351705,0.005017454],"category_scores_gemma":[0.002735944,0.00012582561,0.00024464625,0.0011863308,0.0004254585,0.0006760845,0.0009174402,0.00066078274,0.0010885634],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056140486,0.00012965199,0.23393561,0.00032234774,0.00014155322,0.00017715749,0.00065403787,0.0066063437,0.0050163707,0.29432887,0.2007503,0.25737634],"study_design_scores_gemma":[0.00008674201,0.00014502287,0.45484322,0.00014904689,0.00006005888,0.0005292084,0.00011731895,0.014274255,0.0033309106,0.073421314,0.4529645,0.0000784439],"about_ca_topic_score_codex":0.02226835,"about_ca_topic_score_gemma":0.014640827,"teacher_disagreement_score":0.02226835,"about_ca_system_score_codex":0.0009429281,"about_ca_system_score_gemma":0.0010211144,"threshold_uncertainty_score":0.04427749},"labels":[],"label_agreement":null},{"id":"W1986002430","doi":"10.1086/379156","title":"Interpenetrating Plasma Shells: Near-Equipartition Magnetic Field Generation and Nonthermal Particle Acceleration","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":402,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Equipartition theorem; Particle acceleration; Magnetic field; Relativistic particle; Plasma; Particle-in-cell; Kinetic energy; Particle (ecology); Acceleration; Pulsar; Relativistic plasma; Computational physics; Astrophysics; Electron; Nuclear physics; Classical mechanics; Quantum mechanics","score_opus":0.016093049667813955,"score_gpt":0.23182103590353192,"score_spread":0.21572798623571798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986002430","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9523824,0.00019910511,0.033083104,0.00021464024,0.000065639615,0.000082934166,0.00021932015,0.00024780567,0.013505044],"genre_scores_gemma":[0.99167705,0.00006473483,0.006499899,0.000058373003,0.000013916307,0.00005451703,0.0001293319,0.00006006489,0.0014420525],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986684,0.000032186257,0.0000038056394,0.0000133232925,0.000037217087,0.00004665287],"domain_scores_gemma":[0.9995253,0.0002095899,0.000073436975,0.000041572974,0.00005237519,0.00009776774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030914103,0.00040798166,0.000620049,0.00022881365,0.00066657906,0.0010274397,0.001058341,0.00097040867,0.0019528368],"category_scores_gemma":[0.0019385646,0.00046642794,0.00051805086,0.00032655377,0.0009366058,0.0005952777,0.0008969607,0.00073442765,0.00020503308],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019319195,0.000065656764,0.0028063592,0.000034274086,0.00004213031,0.000353611,0.00016639027,0.9842329,0.0028740172,0.0067488197,0.00029435536,0.0021882572],"study_design_scores_gemma":[0.000089164736,0.000045208297,0.0007262327,0.0000028353115,0.000009192395,0.00004992924,0.000037023918,0.99637187,0.0009400014,0.001252251,0.00046486716,0.000011403575],"about_ca_topic_score_codex":0.009424584,"about_ca_topic_score_gemma":0.00441673,"teacher_disagreement_score":0.009424584,"about_ca_system_score_codex":0.00059973303,"about_ca_system_score_gemma":0.0008088767,"threshold_uncertainty_score":0.018739462},"labels":[],"label_agreement":null},{"id":"W1986083779","doi":"10.1088/0004-637x/753/1/20","title":"MATCHING THE SPECTRAL ENERGY DISTRIBUTION AND<i>p</i>-MODE OSCILLATION FREQUENCIES OF THE RAPIDLY ROTATING DELTA SCUTI STAR α OPHIUCHI WITH A TWO-DIMENSIONAL ROTATING STELLAR MODEL","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Amplitude; Oscillation (cell signaling); Mode (computer interface); Spectral energy distribution; Normal mode; Galaxy; Optics","score_opus":0.010305103053228244,"score_gpt":0.22109932448222877,"score_spread":0.21079422142900053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986083779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973501,0.000010791768,0.0016403439,0.000016005133,0.0000015770428,0.0000067669384,0.00016999958,0.000054616292,0.0007497114],"genre_scores_gemma":[0.9986935,0.00000878125,0.0009105342,0.0000035115468,0.0000012123667,0.0000046942887,0.00025883713,0.000011065576,0.000107815526],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999198,0.000013013188,0.0000055345936,0.000026193271,0.000016386688,0.000019233641],"domain_scores_gemma":[0.9998292,0.00004235824,0.000039716513,0.000029474499,0.00003407718,0.000025239886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024552556,0.00037137393,0.00018910138,0.0005294664,0.0002966956,0.0004886425,0.00037003227,0.00038004806,0.0008110413],"category_scores_gemma":[0.0007865427,0.00018947174,0.00034714057,0.0005730688,0.00019617217,0.00024111186,0.00020898967,0.0001938788,0.00016284973],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005396895,0.00014080199,0.40289673,0.00007513486,0.0001288357,0.0006024123,0.00028877772,0.5293992,0.04876594,0.0031600578,0.00078772736,0.013214695],"study_design_scores_gemma":[0.00007587827,0.00010848712,0.15582968,0.000008511496,0.000024785806,0.00015964301,0.0001449336,0.8362747,0.0061542587,0.0007623416,0.000433675,0.000023091061],"about_ca_topic_score_codex":0.016498996,"about_ca_topic_score_gemma":0.008995948,"teacher_disagreement_score":0.016498996,"about_ca_system_score_codex":0.0006541939,"about_ca_system_score_gemma":0.00031961073,"threshold_uncertainty_score":0.03280592},"labels":[],"label_agreement":null},{"id":"W1986094184","doi":"10.1086/500238","title":"Models of Ultraluminous X‐Ray Sources with Intermediate‐Mass Black Holes","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Stars; Binary number; RADIUS; Population; Luminosity; Stellar evolution; Orbital elements; Star (game theory)","score_opus":0.009446433912146267,"score_gpt":0.20093958827501812,"score_spread":0.19149315436287184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986094184","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9857465,0.000099716715,0.011148324,0.00016192661,0.000012923027,0.000028884426,0.00035492738,0.00009835452,0.0023484689],"genre_scores_gemma":[0.98997515,0.000097525815,0.007953968,0.000048081292,0.000014823837,0.000068417314,0.0005499313,0.00004614532,0.0012459023],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984145,0.000049432234,0.000008739315,0.00003081151,0.000024450668,0.000045108256],"domain_scores_gemma":[0.9990841,0.0004898076,0.00012183788,0.00007048484,0.000093904135,0.0001398898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056849135,0.0005004678,0.00063897274,0.0005278199,0.0007736993,0.0011115998,0.002295355,0.0011826864,0.002040837],"category_scores_gemma":[0.0020654693,0.00062282383,0.00095983886,0.00056194747,0.00072630995,0.0014977433,0.000820514,0.000923815,0.0002037084],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008908408,0.000047656813,0.009890229,0.000015608008,0.00003403129,0.00012447179,0.00009269271,0.9842738,0.00059958844,0.0038403778,0.00017709273,0.0008154648],"study_design_scores_gemma":[0.000047638467,0.000020613465,0.0010472356,0.0000030755023,0.000010060515,0.000028579878,0.00002836926,0.9970509,0.00028357914,0.0012307724,0.00024266823,0.0000064260676],"about_ca_topic_score_codex":0.01969196,"about_ca_topic_score_gemma":0.011300422,"teacher_disagreement_score":0.01969196,"about_ca_system_score_codex":0.0017677256,"about_ca_system_score_gemma":0.0008862578,"threshold_uncertainty_score":0.03915471},"labels":[],"label_agreement":null},{"id":"W1986202073","doi":"10.1086/512230","title":"PROSAC: A Submillimeter Array Survey of Low‐Mass Protostars. I. Overview of Program: Envelopes, Disks, Outflows, and Hot Cores","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":283,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Protostar; Astrophysics; Submillimeter Array; Opacity; Outflow; Millimeter; Basso continuo; Envelope (radar); Accretion (finance); Emission spectrum; Astronomy; Circumstellar disk; Circumstellar envelope; Spectral line; Radiative transfer; Star formation; Stars; Galaxy; Optics","score_opus":0.03522546162426598,"score_gpt":0.29994626510344297,"score_spread":0.264720803479177,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986202073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.74798405,0.0026142234,0.015373918,0.0007236094,0.00012721209,0.00089845376,0.17817135,0.0040838495,0.050023276],"genre_scores_gemma":[0.72396964,0.0019734928,0.047198005,0.0007357292,0.00037842884,0.0010405474,0.20236613,0.0005423758,0.021795662],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997427,0.000047448222,0.000010651601,0.00006908753,0.000073897,0.00005629384],"domain_scores_gemma":[0.99924135,0.00005366307,0.00018238946,0.000092948736,0.00017881379,0.00025089196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006087579,0.00059416756,0.00024031223,0.0033106788,0.0004203714,0.0005770843,0.00051874237,0.00025923064,0.0048516816],"category_scores_gemma":[0.0004419456,0.0002603594,0.00023303917,0.0020348546,0.0001351133,0.0005222995,0.0009615257,0.00034182044,0.0025836392],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034846738,0.00017264573,0.7394464,0.00036564856,0.00020355875,0.00029602117,0.00089289696,0.0007462453,0.030925378,0.0014690459,0.058989882,0.1661439],"study_design_scores_gemma":[0.000018020131,0.00012395388,0.94019353,0.000030342531,0.000024858628,0.00043209936,0.00020768784,0.0010875996,0.0013096485,0.00024797858,0.05631379,0.000010345554],"about_ca_topic_score_codex":0.0073493603,"about_ca_topic_score_gemma":0.010191559,"teacher_disagreement_score":0.0073493603,"about_ca_system_score_codex":0.00028375402,"about_ca_system_score_gemma":0.0005786424,"threshold_uncertainty_score":0.016230464},"labels":[],"label_agreement":null},{"id":"W1986205992","doi":"10.1088/0004-637x/703/1/l6","title":"DETECTION OF EXTENDED VHE GAMMA RAY EMISSION FROM G106.3+2.7 WITH VERITAS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Supernova remnant; Crab Nebula; Astrophysics; Cherenkov radiation; Pulsar wind nebula; Gamma ray; Flux (metallurgy); Astronomy; Context (archaeology); Cherenkov Telescope Array; Vela; Telescope; Nebula; Supernova; Detector; Stars; Optics","score_opus":0.00513802989255184,"score_gpt":0.2035791515631285,"score_spread":0.19844112167057665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986205992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997985,0.00011328359,0.00041882988,0.000019593026,0.000007131442,0.0000061706774,0.00037567556,0.000086435626,0.0009878835],"genre_scores_gemma":[0.9935136,0.00008497662,0.0030027567,0.000052385538,0.000010362693,0.000007540939,0.0027170135,0.000026273741,0.0005852273],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998067,0.000014011111,0.000010385635,0.00004482093,0.00009103463,0.000033040687],"domain_scores_gemma":[0.99968314,0.000035334462,0.00010778782,0.00004862114,0.000053855867,0.000071282615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025101347,0.00020185884,0.00020883747,0.00030387598,0.0001780323,0.00042054476,0.00034113223,0.0002897749,0.0008842511],"category_scores_gemma":[0.00043724373,0.0001315792,0.00019104984,0.00025270157,0.00020798063,0.00015808204,0.0004278425,0.00027647323,0.00030826047],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081556506,0.000102384955,0.37715438,0.000089331465,0.00011522696,0.0015214536,0.00023455736,0.0013074315,0.59011126,0.00045908947,0.0009821646,0.02710711],"study_design_scores_gemma":[0.00007936253,0.0010293332,0.86143035,0.000024387386,0.00009184019,0.0053719147,0.00011280141,0.005117042,0.11687811,0.000353375,0.009470073,0.000041446416],"about_ca_topic_score_codex":0.001377728,"about_ca_topic_score_gemma":0.004000987,"teacher_disagreement_score":0.001377728,"about_ca_system_score_codex":0.0002353711,"about_ca_system_score_gemma":0.00014971073,"threshold_uncertainty_score":0.0029581785},"labels":[],"label_agreement":null},{"id":"W1986325884","doi":"10.1088/0004-637x/776/1/23","title":"GIANT MOLECULAR CLOUD FORMATION IN DISK GALAXIES: CHARACTERIZING SIMULATED VERSUS OBSERVED CLOUD CATALOGS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Star formation; Milky Way; Astrophysics; Molecular cloud; Galaxy; Galactic Center; Astronomy; Cloud computing; Gravitational potential; Population; Star cluster; Stars","score_opus":0.01874324543618125,"score_gpt":0.23441680868247125,"score_spread":0.21567356324629,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986325884","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99919945,0.000026148005,0.00019071244,0.000008897539,3.6329297e-7,0.0000073588026,0.00039240698,0.000016861632,0.00015780097],"genre_scores_gemma":[0.9979711,0.000022387047,0.000336489,0.00000355895,0.0000010688963,0.000006489887,0.0015807898,0.0000064782553,0.00007160084],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998084,0.00004307895,0.00001585031,0.000048376158,0.000034856537,0.000049583243],"domain_scores_gemma":[0.9975426,0.001064031,0.0004823545,0.00031725966,0.00030844376,0.00028532805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006661869,0.00021865989,0.0002193703,0.0012151292,0.00030558978,0.00072085415,0.00062283984,0.00032717825,0.00047497806],"category_scores_gemma":[0.0038855744,0.00014394821,0.00033558838,0.0011612694,0.0003239389,0.00050414156,0.00044159734,0.00012791545,0.00009152358],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017531005,0.00007608969,0.92914623,0.000028363414,0.000059698883,0.00011654147,0.0002475533,0.06383413,0.0020181364,0.00067259505,0.00025333953,0.0033720755],"study_design_scores_gemma":[0.000068879985,0.00017501142,0.605367,0.000017581899,0.000040926807,0.00022408394,0.00036674875,0.3896633,0.0025227892,0.0005962419,0.0009375641,0.0000199367],"about_ca_topic_score_codex":0.022674756,"about_ca_topic_score_gemma":0.021784348,"teacher_disagreement_score":0.022674756,"about_ca_system_score_codex":0.001231787,"about_ca_system_score_gemma":0.00042322703,"threshold_uncertainty_score":0.04508555},"labels":[],"label_agreement":null},{"id":"W1986439752","doi":"10.1088/0004-637x/715/2/897","title":"<i>EXTREME ULTRAVIOLET EXPLORER</i>OBSERVATIONS OF HERCULES X-1 OVER A 35 DAY CYCLE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; University of Calgary","funders":"","keywords":"Physics; Astrophysics; Extreme ultraviolet lithography; Extreme ultraviolet; Flux (metallurgy); Accretion (finance); Ultraviolet; Astronomy; Accretion disc; X-ray; Optics","score_opus":0.024410405321640048,"score_gpt":0.2376293397996724,"score_spread":0.21321893447803236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986439752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96501064,0.0008021047,0.0004136046,0.00048923265,0.00006084585,0.00005800179,0.011901859,0.00055084,0.020712888],"genre_scores_gemma":[0.9729959,0.0003530481,0.0017837582,0.00028644278,0.00013344451,0.000037874997,0.019190129,0.00009755414,0.005121929],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999025,0.000008951717,0.000005319699,0.00002049391,0.000034557477,0.000028069908],"domain_scores_gemma":[0.9997149,0.000021775395,0.00009966979,0.00004399091,0.000046318364,0.00007328396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018622185,0.00022233643,0.0001844844,0.0016195015,0.00053583825,0.00045499444,0.00027158667,0.00025757236,0.0033308119],"category_scores_gemma":[0.0002631432,0.00010207047,0.000116949675,0.00082973944,0.00013752369,0.00017169789,0.00059000624,0.00029308096,0.0006358202],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015320636,0.00044274583,0.6130804,0.00036523625,0.0003478577,0.0033956815,0.0009776634,0.0033568183,0.14856192,0.0017220149,0.11645884,0.10975871],"study_design_scores_gemma":[0.000022126644,0.00006307852,0.9731799,0.000019968722,0.000015155948,0.0004548971,0.000059018563,0.0004256682,0.0026106068,0.00012619163,0.023008816,0.000014667083],"about_ca_topic_score_codex":0.008279864,"about_ca_topic_score_gemma":0.023797229,"teacher_disagreement_score":0.008279864,"about_ca_system_score_codex":0.00040517576,"about_ca_system_score_gemma":0.00016305404,"threshold_uncertainty_score":0.01646334},"labels":[],"label_agreement":null},{"id":"W1986459807","doi":"10.1088/0004-637x/747/2/145","title":"NEW EVIDENCE SUPPORTING CLUSTER MEMBERSHIP FOR THE KEYSTONE CALIBRATOR DELTA CEPHEI","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Cepheid variable; Physics; Astrophysics; Hubble space telescope; Cluster (spacecraft); Stars; Instability strip; Supergiant; Open cluster; Star cluster; Astronomy; Star (game theory); Magnitude (astronomy); Computer science","score_opus":0.03487575422088797,"score_gpt":0.28221948840980826,"score_spread":0.2473437341889203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986459807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99292094,0.0002374026,0.00076641736,0.00015525488,0.000035346395,0.000008378084,0.0002155774,0.000025241929,0.005635465],"genre_scores_gemma":[0.998803,0.000059104917,0.00032660124,0.0000422704,0.0000135616665,0.0000025975971,0.00024988447,0.000005028241,0.00049795996],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970406,0.000019366655,0.000021220874,0.0000967909,0.000091444235,0.00006709889],"domain_scores_gemma":[0.99684286,0.00064174033,0.00066217827,0.0005124201,0.000686869,0.0006539668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006463141,0.00014220495,0.00022951304,0.0013067225,0.000968565,0.00091102475,0.00073978264,0.0003006023,0.0042095874],"category_scores_gemma":[0.0028325864,0.0001244104,0.00009051918,0.00087328703,0.00064675533,0.00045519415,0.0007440623,0.00035238505,0.0003884912],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002530969,0.000028501929,0.9757134,0.000050925926,0.000042534666,0.00044417815,0.0009553763,0.00016911098,0.007709622,0.0024314863,0.0010973697,0.011104343],"study_design_scores_gemma":[0.000011686729,0.000050353203,0.99062,0.000030419258,0.00004075394,0.0007520755,0.0010136688,0.00083902373,0.0012330009,0.00069376046,0.0047035394,0.000011642265],"about_ca_topic_score_codex":0.01130013,"about_ca_topic_score_gemma":0.021924239,"teacher_disagreement_score":0.01130013,"about_ca_system_score_codex":0.0005889168,"about_ca_system_score_gemma":0.0005224922,"threshold_uncertainty_score":0.022468686},"labels":[],"label_agreement":null},{"id":"W1986613795","doi":"10.1086/512010","title":"Massive Star Formation via High Accretion Rates and Early Disk‐driven Outflows","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Protostar; Gravitational collapse; Star formation; Accretion (finance); Radiation pressure; Stars; Molecular cloud; Accretion disc; High mass","score_opus":0.007647719976089535,"score_gpt":0.2341171157340416,"score_spread":0.22646939575795205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986613795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99796695,0.00003881251,0.0013949585,0.000019808296,0.0000024316187,0.0000046245123,0.000011102783,0.000023488188,0.0005378536],"genre_scores_gemma":[0.999395,0.000026546713,0.000450689,0.000005556847,0.000002558026,0.0000028776683,0.00001172366,0.0000041958083,0.00010091513],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999306,0.000022390672,0.0000031582638,0.000009314791,0.000014450742,0.000020172727],"domain_scores_gemma":[0.99964666,0.000111783535,0.000120000135,0.000029201667,0.00002871567,0.00006358868],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002466358,0.00032211174,0.00026288268,0.00016434507,0.0003460046,0.00062398624,0.00043134834,0.00037107858,0.00036720655],"category_scores_gemma":[0.0012806022,0.00023646408,0.00029118455,0.00011906921,0.0005582686,0.00033455883,0.00044048595,0.0003071712,0.00006535224],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000545869,0.00025786008,0.057797994,0.00008765888,0.00015104424,0.0016784255,0.000388484,0.833659,0.09028736,0.010522985,0.00025816445,0.0043651825],"study_design_scores_gemma":[0.00015475007,0.00023291542,0.020867921,0.0000086721975,0.00003708155,0.00018722705,0.000063831234,0.96554446,0.010448584,0.0020643775,0.00036985113,0.000020384303],"about_ca_topic_score_codex":0.0034496593,"about_ca_topic_score_gemma":0.001578268,"teacher_disagreement_score":0.0034496593,"about_ca_system_score_codex":0.00058704254,"about_ca_system_score_gemma":0.00030156164,"threshold_uncertainty_score":0.0068591237},"labels":[],"label_agreement":null},{"id":"W1986691938","doi":"10.1088/0004-637x/768/2/128","title":"A CHARA ARRAY SURVEY OF CIRCUMSTELLAR DISKS AROUND NEARBY Be-TYPE STARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":227,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Position angle; Stars; Opacity; Angular diameter; Astronomy; Angular resolution (graph drawing); Sky; Flux (metallurgy); Optics; Galaxy","score_opus":0.024398001726353577,"score_gpt":0.24138929005532758,"score_spread":0.21699128832897402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986691938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975585,0.00010844711,0.0002938369,0.00002786648,0.0000028221955,0.000008849696,0.0005853302,0.00003439722,0.0013799815],"genre_scores_gemma":[0.9945229,0.00010806937,0.0018084525,0.000028117744,0.00001929497,0.000010138086,0.0026155047,0.00001287744,0.0008746164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967146,0.000054835687,0.000016734757,0.00009334441,0.0001076173,0.000056116387],"domain_scores_gemma":[0.9988016,0.00008301481,0.00018927656,0.00013101955,0.00027044697,0.00052469375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046319683,0.0002129779,0.0002789313,0.0015795948,0.0008625564,0.0005755147,0.0002291551,0.00024818582,0.00082304643],"category_scores_gemma":[0.0006088638,0.00015926732,0.0001614745,0.000997512,0.00019456477,0.00032634835,0.00062721013,0.00022864291,0.0005190349],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020981516,0.0001439708,0.93978727,0.000044639604,0.00005994148,0.0005388199,0.0004575252,0.0004582107,0.0381516,0.0001525022,0.00090218656,0.019093435],"study_design_scores_gemma":[0.000009043498,0.00010672081,0.9945028,0.000004109244,0.000015460664,0.00058829936,0.00013401742,0.00071724266,0.0013419673,0.000045304634,0.0025283603,0.0000067052624],"about_ca_topic_score_codex":0.0032609769,"about_ca_topic_score_gemma":0.009121736,"teacher_disagreement_score":0.0032609769,"about_ca_system_score_codex":0.00022563762,"about_ca_system_score_gemma":0.0003191984,"threshold_uncertainty_score":0.006483972},"labels":[],"label_agreement":null},{"id":"W1986751435","doi":"10.1088/0004-637x/716/1/234","title":"THE DISKMASS SURVEY. II. ERROR BUDGET","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Halo; Measure (data warehouse); Galaxy; Rotation (mathematics); Galaxy rotation curve; Thick disk; Scale (ratio); Stars; Calibration; Spiral galaxy","score_opus":0.008098777952739052,"score_gpt":0.22596901708469375,"score_spread":0.2178702391319547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1986751435","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.18919367,0.00475143,0.1607896,0.002123574,0.00033470534,0.00097157387,0.5914103,0.012174901,0.038250238],"genre_scores_gemma":[0.39648992,0.0020980889,0.15081552,0.00095153454,0.0003290875,0.0012263437,0.42447528,0.0031417743,0.020472357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99325365,0.0018379503,0.0006231911,0.0016363991,0.0022968925,0.00035186615],"domain_scores_gemma":[0.9793467,0.0051907306,0.0034121973,0.00571614,0.00596809,0.00036609903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0096849045,0.0011851601,0.0006152974,0.00446154,0.0004363943,0.0017602133,0.0018158254,0.0007878288,0.0066629983],"category_scores_gemma":[0.028903035,0.00049166445,0.00050859456,0.0061615943,0.00041203343,0.0018504234,0.001633701,0.0005170107,0.008660149],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069968414,0.00012762476,0.5093697,0.00070738554,0.0005116547,0.000105222425,0.0002496037,0.027116934,0.0030690718,0.014863318,0.10554495,0.3376349],"study_design_scores_gemma":[0.00017543983,0.000177268,0.46034604,0.00053485925,0.00025153687,0.00074041146,0.0003584841,0.07546124,0.014748587,0.020511685,0.42651632,0.00017808404],"about_ca_topic_score_codex":0.02358614,"about_ca_topic_score_gemma":0.014230491,"teacher_disagreement_score":0.02358614,"about_ca_system_score_codex":0.0017367227,"about_ca_system_score_gemma":0.0010282838,"threshold_uncertainty_score":0.051219285},"labels":[],"label_agreement":null},{"id":"W1987005932","doi":"10.1086/516730","title":"Protoplanetary Disk Turbulence Driven by the Streaming Instability: Nonlinear Saturation and Particle Concentration","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":468,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Turbulence; Physics; Mechanics; Drag; Streaming instability; Laminar flow; Planetesimal; Instability; Protoplanetary disk; Accretion (finance); Saturation (graph theory); Particle (ecology); Astrophysics; Planet","score_opus":0.007354107958835843,"score_gpt":0.22980925111470715,"score_spread":0.2224551431558713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987005932","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99696976,0.000037938404,0.000992614,0.00009079814,0.000006677254,0.000009710169,0.000056276265,0.000037158192,0.0017990717],"genre_scores_gemma":[0.9991567,0.000019549769,0.00046101585,0.000013255692,0.0000031754187,0.000007197008,0.000049969854,0.000011046304,0.00027798428],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999182,0.000017583372,0.0000039064976,0.000011052171,0.00001653282,0.00003265108],"domain_scores_gemma":[0.9995223,0.00020120242,0.00007589705,0.000024807334,0.000052562224,0.00012325372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018937892,0.0004189594,0.00040384656,0.00028936082,0.0005608813,0.00072038174,0.0006703684,0.00072284497,0.0010240356],"category_scores_gemma":[0.0012561897,0.0002361948,0.00044018056,0.00031087536,0.0009487053,0.00051625184,0.0006992062,0.0005576988,0.00009139372],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035236843,0.00015546683,0.014101924,0.000038052993,0.00004062152,0.00030003645,0.00015396025,0.9738912,0.0060976343,0.0029674887,0.00029650956,0.0016047463],"study_design_scores_gemma":[0.000056766137,0.000043860746,0.0014789817,0.0000024281192,0.0000057545617,0.000013424248,0.000033229422,0.9971819,0.0006999542,0.00040973793,0.000067712295,0.000006251398],"about_ca_topic_score_codex":0.027433127,"about_ca_topic_score_gemma":0.0101518035,"teacher_disagreement_score":0.027433127,"about_ca_system_score_codex":0.0011063088,"about_ca_system_score_gemma":0.0006613406,"threshold_uncertainty_score":0.054546893},"labels":[],"label_agreement":null},{"id":"W1987106004","doi":"10.1088/0004-637x/707/2/1824","title":"BLAST: THE MASS FUNCTION, LIFETIMES, AND PROPERTIES OF INTERMEDIATE MASS CORES FROM A 50 deg<sup>2</sup>SUBMILLIMETER GALACTIC SURVEY IN VELA (ℓ ≈ 265°)","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of British Columbia; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Vela; Astronomy; Submillimeter Array; Telescope; Population; Star formation; Opacity; Luminosity; High mass; Millimeter; Galaxy; Pulsar","score_opus":0.015521265152719326,"score_gpt":0.21324108702309996,"score_spread":0.19771982187038065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987106004","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975757,0.000102652855,0.00023626137,0.000013430011,0.0000013976212,0.0000040816153,0.0015877639,0.000028513905,0.00045022328],"genre_scores_gemma":[0.9932307,0.00008239904,0.00074987777,0.000022693019,0.0000110881665,0.0000061091414,0.005401669,0.0000196862,0.00047577842],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998702,0.000015527334,0.00000989424,0.000037333954,0.00003138954,0.00003565228],"domain_scores_gemma":[0.99936515,0.000054780317,0.0002629388,0.00006218301,0.00009018054,0.00016473663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002739564,0.00022215545,0.00024987638,0.0011630356,0.0002334584,0.00044108136,0.00040846094,0.00021245726,0.00075193093],"category_scores_gemma":[0.00045784286,0.00023058013,0.00020040633,0.00093274214,0.00018961885,0.00024488172,0.0004808861,0.00018504357,0.00041743176],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007996845,0.000014780014,0.9878405,0.000014492704,0.000045465382,0.000081712285,0.00020107249,0.00018678993,0.0065460377,0.00004723591,0.0005375152,0.0044044694],"study_design_scores_gemma":[0.000002172084,0.00001232579,0.99905735,0.0000017004812,0.0000075766843,0.00006167587,0.000043364893,0.00018194209,0.000275435,0.000009201134,0.00034575278,0.0000015306031],"about_ca_topic_score_codex":0.017413652,"about_ca_topic_score_gemma":0.04997849,"teacher_disagreement_score":0.017413652,"about_ca_system_score_codex":0.00037928476,"about_ca_system_score_gemma":0.00015644963,"threshold_uncertainty_score":0.034624577},"labels":[],"label_agreement":null},{"id":"W1987130167","doi":"10.1088/0004-637x/748/1/56","title":"WEAK LENSING MEASUREMENT OF GALAXY CLUSTERS IN THE CFHTLS-WIDE SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Centre National de la Recherche Scientifique; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Weak gravitational lensing; Redshift; Galaxy; Gravitational lens; Velocity dispersion; Strong gravitational lensing; Galaxy cluster; Redshift survey; Einstein radius","score_opus":0.024859092693490785,"score_gpt":0.22959610279771012,"score_spread":0.20473701010421932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987130167","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945714,0.00008599673,0.0005121853,0.000047916,0.0000030219564,0.000017608661,0.0029229426,0.000051755378,0.001787202],"genre_scores_gemma":[0.99254674,0.00004764889,0.0012841206,0.000028733613,0.000011215166,0.00001608016,0.005626359,0.000011763508,0.0004272209],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995608,0.00003806349,0.000016987982,0.000093094866,0.00016778821,0.00012318477],"domain_scores_gemma":[0.99745923,0.00018545776,0.00039958372,0.00026398155,0.00087884744,0.0008130165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006301383,0.0003081723,0.00020596833,0.0030086907,0.00083079364,0.0005034323,0.00039794706,0.00017788282,0.0012764612],"category_scores_gemma":[0.0021877133,0.00014397774,0.00019206482,0.0016270153,0.00037825998,0.00033059338,0.0010304924,0.0002678046,0.00028428502],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003927601,0.000017441193,0.9867993,0.000012310973,0.00004097397,0.000052333835,0.00031148724,0.0004287016,0.0037418113,0.00018008065,0.0012573869,0.0071188547],"study_design_scores_gemma":[0.0000020834368,0.000011805702,0.99824476,0.0000023651407,0.000007638329,0.000025811367,0.00006736229,0.0005020801,0.00036978596,0.000021019163,0.00074102415,0.000004359791],"about_ca_topic_score_codex":0.31835246,"about_ca_topic_score_gemma":0.43130535,"teacher_disagreement_score":0.31835246,"about_ca_system_score_codex":0.0017455609,"about_ca_system_score_gemma":0.0012151673,"threshold_uncertainty_score":0.6329989},"labels":[],"label_agreement":null},{"id":"W1987197986","doi":"10.1088/0004-637x/768/1/58","title":"H-ATLAS: THE COSMIC ABUNDANCE OF DUST FROM THE FAR-INFRARED BACKGROUND POWER SPECTRUM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Aeronautics and Space Administration; Science and Technology Facilities Council; National Science Foundation","keywords":"Astronomy; COSMIC cancer database; Cosmic infrared background; Far infrared; Atlas (anatomy); Physics; Abundance (ecology); Infrared; Astrophysics; Cosmic ray; Environmental science; Astrobiology; Cosmic microwave background; Geology; Optics; Ecology; Biology","score_opus":0.007531393546981262,"score_gpt":0.20208110506463683,"score_spread":0.19454971151765557,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987197986","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.102922685,0.0016318515,0.026872171,0.0003595386,0.0003666234,0.00020677244,0.76766306,0.023464244,0.07651301],"genre_scores_gemma":[0.32424,0.0007915259,0.030420097,0.00030421748,0.00027689032,0.0002569614,0.6299048,0.0020671643,0.011738379],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996573,0.00003801826,0.000015144931,0.000087844994,0.00015695438,0.00004473528],"domain_scores_gemma":[0.99918014,0.00008900445,0.00016607458,0.00014599059,0.00027747458,0.00014131202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037275103,0.00067362405,0.00046819128,0.0023594282,0.00029502323,0.0010400862,0.00089785416,0.00029549445,0.0119715445],"category_scores_gemma":[0.0010089619,0.00023199899,0.00036565604,0.0020024478,0.00020516646,0.00079079496,0.0007061845,0.00042728,0.006580716],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011309165,0.00014054772,0.17574751,0.00089183234,0.00059019733,0.000353861,0.0003826919,0.00878361,0.01810961,0.0142448,0.6535211,0.1261033],"study_design_scores_gemma":[0.00018320448,0.0001327503,0.51208955,0.000115013296,0.00016515763,0.00071705563,0.00017746528,0.015586023,0.016618878,0.008560106,0.44551188,0.0001428373],"about_ca_topic_score_codex":0.01568391,"about_ca_topic_score_gemma":0.018501025,"teacher_disagreement_score":0.01568391,"about_ca_system_score_codex":0.0005764359,"about_ca_system_score_gemma":0.0004218173,"threshold_uncertainty_score":0.040048778},"labels":[],"label_agreement":null},{"id":"W1987199236","doi":"10.1086/308293","title":"Consistency of Ambipolar Diffusion Models with Infall in the L1544 Protostellar Core","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Western University","funders":"","keywords":"Ambipolar diffusion; Core (optical fiber); Diffusion; Consistency (knowledge bases); Magnetic field; Kinematics; Inner core","score_opus":0.014666934334613517,"score_gpt":0.22625100216840968,"score_spread":0.21158406783379616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987199236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98693126,0.00017800338,0.009416748,0.00039430472,0.000012018065,0.00001904482,0.00010137192,0.000077568235,0.0028696293],"genre_scores_gemma":[0.9988098,0.000088126566,0.0006461756,0.00003628547,0.000010276568,0.000009245944,0.00006816924,0.000016167667,0.0003159231],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99975544,0.00007445829,0.00002211096,0.000061342296,0.000030327019,0.000056329038],"domain_scores_gemma":[0.9989188,0.00050270546,0.0002627369,0.00009339733,0.000102776256,0.0001196765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007747709,0.00067409605,0.00057576655,0.0006576508,0.00058191246,0.0012320653,0.0011527945,0.00086525024,0.000774102],"category_scores_gemma":[0.0041612205,0.0006338883,0.00061157666,0.0002512306,0.0009891748,0.0012501136,0.0011572796,0.00033489295,0.00015578348],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003728388,0.00008197258,0.030760601,0.000030334599,0.000111808724,0.0003819938,0.00015535262,0.94734424,0.003510183,0.014520721,0.00035502526,0.0023750237],"study_design_scores_gemma":[0.00009205049,0.000033617875,0.0031569116,0.0000033185884,0.000019186864,0.000052003175,0.000038542683,0.9908635,0.00048714565,0.0050865766,0.00015173088,0.00001539501],"about_ca_topic_score_codex":0.020021565,"about_ca_topic_score_gemma":0.006575307,"teacher_disagreement_score":0.020021565,"about_ca_system_score_codex":0.0012730531,"about_ca_system_score_gemma":0.00054859923,"threshold_uncertainty_score":0.03981006},"labels":[],"label_agreement":null},{"id":"W1987239612","doi":"10.1088/0004-637x/761/2/150","title":"MEASURING THE ABUNDANCE OF SUB-KILOMETER-SIZED KUIPER BELT OBJECTS USING STELLAR OCCULTATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Ecliptic; Occultation; Latitude; RADIUS; Stars; Event (particle physics); Magnitude (astronomy)","score_opus":0.030813041070031785,"score_gpt":0.2471760194389245,"score_spread":0.21636297836889273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987239612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986576,0.00008366317,0.0005277595,0.0000060835005,0.0000022454215,0.0000041611083,0.00017882662,0.000015041595,0.0005246814],"genre_scores_gemma":[0.9981799,0.000061214734,0.0010643676,0.000007804975,0.000009867533,0.0000057277116,0.00046120404,0.0000050495323,0.00020477196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998393,0.00001580431,0.000008990951,0.000064338004,0.000047300542,0.000024296412],"domain_scores_gemma":[0.998585,0.00033048834,0.0006627039,0.00011661308,0.00011610407,0.00018917669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020783771,0.00020190736,0.00017765262,0.000933743,0.00021818069,0.00039902114,0.00029541357,0.00018142466,0.00081497955],"category_scores_gemma":[0.0010911162,0.0001387574,0.00014905706,0.0005558263,0.00022085091,0.00046197145,0.00038845712,0.00017484967,0.00035861644],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000610297,0.000012589219,0.98598796,0.000011014157,0.000030121673,0.000070271155,0.0001573964,0.00032188513,0.008460278,0.000032824548,0.00006184528,0.0047928556],"study_design_scores_gemma":[0.0000013072968,0.000018173167,0.9982432,0.0000013166695,0.000008750695,0.000105009705,0.000039617677,0.0005530412,0.0007850711,0.0000147838555,0.00022714479,0.0000025593065],"about_ca_topic_score_codex":0.002702357,"about_ca_topic_score_gemma":0.009679596,"teacher_disagreement_score":0.002702357,"about_ca_system_score_codex":0.00022400037,"about_ca_system_score_gemma":0.00007874816,"threshold_uncertainty_score":0.0053732395},"labels":[],"label_agreement":null},{"id":"W1987265672","doi":"10.1088/0004-637x/745/1/32","title":"THE<i>HUBBLE SPACE TELESCOPE</i>CLUSTER SUPERNOVA SURVEY. II. THE TYPE Ia SUPERNOVA RATE IN HIGH-REDSHIFT GALAXY CLUSTERS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Supernova; Galaxy; Cluster (spacecraft); Hubble space telescope; Stars; Galaxy cluster; Type (biology); Star cluster","score_opus":0.01771140672800698,"score_gpt":0.23310841355460857,"score_spread":0.2153970068266016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987265672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5350702,0.007120768,0.004833817,0.002135867,0.0005948844,0.0005050474,0.38050458,0.0015983041,0.06763656],"genre_scores_gemma":[0.5942688,0.0071983193,0.00866536,0.0009687081,0.00057568646,0.00047687822,0.3444415,0.00032423373,0.043080494],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996972,0.000034702352,0.000018143852,0.00006671667,0.00012040308,0.00006288586],"domain_scores_gemma":[0.9978561,0.00011918809,0.0006898604,0.00019253224,0.00050049776,0.00064182276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071563234,0.00048195306,0.00023011432,0.0035576038,0.00038336654,0.00053740677,0.0004820815,0.00026520298,0.003980222],"category_scores_gemma":[0.0010912691,0.00018801224,0.00030063358,0.002173641,0.00027968598,0.00037743634,0.000703512,0.0004397685,0.0031632998],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002415082,0.00007899224,0.83432615,0.00020137875,0.00018083781,0.00010995987,0.0001678654,0.0007988395,0.003434639,0.0017739016,0.096406996,0.062278897],"study_design_scores_gemma":[0.000015249787,0.000032527852,0.9615525,0.000034765453,0.000022827959,0.00006414751,0.000024477073,0.0002553585,0.00048770962,0.0001205974,0.037382696,0.0000070986985],"about_ca_topic_score_codex":0.07690493,"about_ca_topic_score_gemma":0.11072273,"teacher_disagreement_score":0.07690493,"about_ca_system_score_codex":0.0011665762,"about_ca_system_score_gemma":0.0010385381,"threshold_uncertainty_score":0.15291458},"labels":[],"label_agreement":null},{"id":"W1987292496","doi":"10.1086/520575","title":"A Compact Cluster of Massive Red Galaxies at a Redshift of 1.5","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Brightest cluster galaxy; Astronomy; Galaxy cluster; Elliptical galaxy; Galaxy group; Redshift; Galaxy; Lenticular galaxy; Luminous infrared galaxy","score_opus":0.008323012974292143,"score_gpt":0.2263658446281434,"score_spread":0.21804283165385127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987292496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9856489,0.0008373935,0.0018071968,0.00024697525,0.000031680378,0.000036566238,0.0007198438,0.00013468521,0.010536837],"genre_scores_gemma":[0.99395895,0.00014947222,0.0014358847,0.000072903305,0.000038672013,0.000006829466,0.00060575234,0.0000072353323,0.003724336],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999485,0.0000019722238,0.0000015501997,0.000015211625,0.000013218245,0.000019550112],"domain_scores_gemma":[0.9998728,0.0000066781517,0.000037253278,0.000008411982,0.000008189362,0.00006661223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000058540438,0.00020584288,0.00017945797,0.00062339066,0.0005208687,0.0005376716,0.00039299374,0.0003122024,0.0024607142],"category_scores_gemma":[0.00014756384,0.000074435884,0.00011267494,0.00048408756,0.00029637612,0.00032743724,0.00050929387,0.00014404599,0.0005658994],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013448012,0.00041462533,0.6731193,0.00043825334,0.00014759452,0.020291654,0.0034830896,0.003949288,0.11283816,0.04320473,0.023257466,0.11751113],"study_design_scores_gemma":[0.0000435409,0.00036941038,0.9044422,0.00006091973,0.000085672014,0.014847022,0.0007967835,0.003533361,0.0057986695,0.0054024034,0.06456095,0.000059165493],"about_ca_topic_score_codex":0.003672246,"about_ca_topic_score_gemma":0.0038618976,"teacher_disagreement_score":0.003672246,"about_ca_system_score_codex":0.00026777908,"about_ca_system_score_gemma":0.00015198578,"threshold_uncertainty_score":0.008231938},"labels":[],"label_agreement":null},{"id":"W1987298753","doi":"10.1088/0004-637x/693/2/1250","title":"THE OUTER DISK OF THE MILKY WAY SEEN IN λ21 cm ABSORPTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Dominion Astrophysical Observatory","funders":"","keywords":"Milky Way; Physics; Astrophysics; Galactic plane; RADIUS; Interstellar medium; Spectral line; Absorption (acoustics); Galaxy; Astronomy; Optics","score_opus":0.007909377750832869,"score_gpt":0.23000297537555905,"score_spread":0.2220935976247262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987298753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975108,0.00017122067,0.00008051398,0.000025727411,0.0000028005584,0.0000027136282,0.00025507962,0.000017120949,0.0019340521],"genre_scores_gemma":[0.99858534,0.00008593627,0.0001544459,0.0000137809,0.0000068180666,0.000002698101,0.0004472483,0.0000066503458,0.000697074],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999238,0.0000048086586,0.0000038452836,0.000029981577,0.0000141221435,0.000023501612],"domain_scores_gemma":[0.99983466,0.000014633629,0.00006956922,0.000016933913,0.000019492896,0.000044545108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007746036,0.00018370082,0.00018420843,0.00064251065,0.00044475606,0.00060945336,0.00028202307,0.00028306877,0.0019385371],"category_scores_gemma":[0.0003238527,0.00012036328,0.00015477503,0.00066743407,0.0002563303,0.0005180577,0.00093836675,0.00010696067,0.00041190797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005940305,0.000088272354,0.85176164,0.000150333,0.0001340313,0.0027120514,0.0038274697,0.0006846175,0.10253195,0.0013593273,0.0015512032,0.034605093],"study_design_scores_gemma":[0.0000038605745,0.00002592714,0.995817,0.0000044841654,0.000010437876,0.00040556872,0.00032299038,0.000105004525,0.000633319,0.00008973337,0.002578044,0.0000036765562],"about_ca_topic_score_codex":0.003321689,"about_ca_topic_score_gemma":0.0049857153,"teacher_disagreement_score":0.003321689,"about_ca_system_score_codex":0.00030941318,"about_ca_system_score_gemma":0.00012563523,"threshold_uncertainty_score":0.0066046715},"labels":[],"label_agreement":null},{"id":"W1987348923","doi":"10.1088/0004-637x/783/1/21","title":"DOES THE DEBRIS DISK AROUND HD 32297 CONTAIN COMETARY GRAINS?,","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Debris disk; Debris; Brightness; Surface brightness; Circumstellar disk; Infrared; Thick disk; Water ice; Scattering","score_opus":0.008394794233673359,"score_gpt":0.21629327628715042,"score_spread":0.20789848205347705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987348923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99718505,0.00028707762,0.0004018841,0.00017999981,0.000009328561,0.000007131246,0.00042870987,0.000039246104,0.0014617256],"genre_scores_gemma":[0.99844176,0.00008464205,0.0004023971,0.000096324606,0.000022011469,0.0000041324106,0.0006698382,0.000015980015,0.0002629818],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991846,0.0000039956844,0.000004275859,0.00003102992,0.000022177164,0.000020090501],"domain_scores_gemma":[0.9997763,0.000036912254,0.00008966663,0.00003741859,0.000025328247,0.00003440876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020062772,0.00023091146,0.00043081125,0.00049718504,0.0005643301,0.0009224873,0.00068898516,0.00095483044,0.0015248096],"category_scores_gemma":[0.00057371776,0.00021544761,0.00027785657,0.0004978141,0.0004896711,0.00063133397,0.00038114635,0.00029378064,0.0008993179],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005946642,0.0001333291,0.8577187,0.00025758948,0.00016476528,0.0029373514,0.00082618056,0.0016516844,0.11430807,0.00075340545,0.0022549897,0.018399356],"study_design_scores_gemma":[0.000044391272,0.00009763384,0.9784695,0.00003753359,0.00007347507,0.0010115545,0.00070945005,0.008349724,0.007772655,0.00048627856,0.0029234842,0.000024250292],"about_ca_topic_score_codex":0.0056157904,"about_ca_topic_score_gemma":0.0074362517,"teacher_disagreement_score":0.0056157904,"about_ca_system_score_codex":0.0006084733,"about_ca_system_score_gemma":0.00015998223,"threshold_uncertainty_score":0.011166215},"labels":[],"label_agreement":null},{"id":"W1987359812","doi":"10.1086/422751","title":"Anomalous X-Ray Pulsar 1E 1048.1-5937: Pulsed Flux Flares and Large Torque Variations","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Flare; Flux (metallurgy); Magnetar; Astronomy; Neutron star; X-ray pulsar","score_opus":0.007740081235874773,"score_gpt":0.2850277504678583,"score_spread":0.2772876692319835,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987359812","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99900985,0.0001340511,0.00018822991,0.000017595268,0.0000038861017,0.000005148509,0.00012300821,0.000019169902,0.0004989673],"genre_scores_gemma":[0.99894255,0.000057518148,0.00047997065,0.000014572854,0.000012958311,0.0000046218956,0.00032398375,0.0000064999035,0.00015732933],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999841,0.000013921338,0.000014006781,0.000040155497,0.000056827263,0.000034029876],"domain_scores_gemma":[0.99934465,0.00010521894,0.000315769,0.00006165173,0.00008653761,0.000086124724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028207386,0.00020778163,0.00038476128,0.00071323063,0.00029705875,0.0004319526,0.0002982779,0.0002448873,0.00054191553],"category_scores_gemma":[0.00086629216,0.00010370033,0.00015133979,0.00064986787,0.00024088022,0.0002180266,0.00029477413,0.00028374078,0.00020269587],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035447325,0.000093765055,0.86710334,0.000060575887,0.00006818132,0.002078625,0.00018627838,0.0005257752,0.10307555,0.00022961543,0.0003718403,0.02585209],"study_design_scores_gemma":[0.000010909102,0.00021648062,0.9906501,0.0000064415344,0.000025862666,0.0022592484,0.000047644728,0.00090693694,0.0049968613,0.00011919926,0.0007504548,0.000009852733],"about_ca_topic_score_codex":0.0010819008,"about_ca_topic_score_gemma":0.0020830878,"teacher_disagreement_score":0.0010819008,"about_ca_system_score_codex":0.00019363938,"about_ca_system_score_gemma":0.00007351439,"threshold_uncertainty_score":0.0021511912},"labels":[],"label_agreement":null},{"id":"W1987365402","doi":"10.1088/0004-637x/778/2/86","title":"DIFFUSE INTERSTELLAR BAND AT 8620 Å IN RAVE: A NEW METHOD FOR DETECTING THE DIFFUSE INTERSTELLAR BAND IN SPECTRA OF COOL STARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leibniz-Gemeinschaft; Science and Technology Facilities Council; Leibniz-Institut für Astrophysik Potsdam; W. M. Keck Foundation; Agence Nationale de la Recherche; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Physics; Stars; Astrophysics; Spectral line; Extinction (optical mineralogy); Interstellar medium; Galaxy; Equivalent width; Radial velocity; Astronomy; Astronomical spectroscopy; Emission spectrum; Optics","score_opus":0.013461553678522267,"score_gpt":0.250952336855838,"score_spread":0.23749078317731576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987365402","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6810584,0.001951434,0.29578188,0.00005752768,0.000051489442,0.0001013131,0.004995032,0.008616362,0.0073866374],"genre_scores_gemma":[0.79052454,0.00034659347,0.19930825,0.000044303015,0.000043221222,0.00006267378,0.006851683,0.0006466431,0.002172019],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9996463,0.000031286465,0.000018405735,0.00018450295,0.00008838326,0.000031133062],"domain_scores_gemma":[0.99959546,0.000047022688,0.00012237046,0.00009358287,0.00008684857,0.00005471274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043083032,0.00047047267,0.00024517794,0.0024578434,0.00012592223,0.0004981044,0.00047735378,0.00039085827,0.0015265862],"category_scores_gemma":[0.0008557828,0.00019313618,0.0005300167,0.00092533947,0.00014853367,0.00053680106,0.0005926602,0.00028094018,0.00094108016],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006724414,0.00027424487,0.26324618,0.00048347327,0.000816004,0.00031509,0.00041344948,0.017906949,0.340651,0.0031385003,0.004801903,0.36728084],"study_design_scores_gemma":[0.000044773846,0.00014539066,0.81024194,0.00005409117,0.00023354878,0.0011780615,0.000116339696,0.09701798,0.07059467,0.0013918278,0.018874913,0.000106525404],"about_ca_topic_score_codex":0.0011217186,"about_ca_topic_score_gemma":0.0015291774,"teacher_disagreement_score":0.0024578434,"about_ca_system_score_codex":0.000121575955,"about_ca_system_score_gemma":0.000112433336,"threshold_uncertainty_score":0.0051069856},"labels":[],"label_agreement":null},{"id":"W1987452328","doi":"10.1086/518209","title":"Star Counts in the Globular Cluster ω Centauri. I. Bright Stellar Components","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Stars; Globular cluster; Subgiant; Metallicity; Horizontal branch; Star cluster; Astronomy; Photometry (optics); Blue straggler; Red-giant branch","score_opus":0.011699530734549863,"score_gpt":0.23081696312825753,"score_spread":0.21911743239370768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987452328","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9862365,0.0010912139,0.00016847151,0.00014217063,0.00004053168,0.000008168856,0.0074855303,0.00006672712,0.00476073],"genre_scores_gemma":[0.9917619,0.0002033663,0.00013787934,0.000033788136,0.000039041708,0.0000064595474,0.0060099065,0.000021573449,0.0017860022],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997291,0.00003870978,0.000023002207,0.00009787743,0.000045651042,0.00006564609],"domain_scores_gemma":[0.99882597,0.00027166025,0.00028178992,0.00011997276,0.00014994865,0.0003506618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049732847,0.00024635685,0.00021433464,0.003632411,0.00040208214,0.0007663691,0.00037280662,0.00032419778,0.0030729368],"category_scores_gemma":[0.001977841,0.00020216586,0.00014213866,0.0021657764,0.0004279279,0.00031177708,0.0009185257,0.0003076753,0.001395731],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015473708,0.00001644616,0.98847187,0.000022593706,0.00002470941,0.00008353866,0.00020093868,0.00022011122,0.0008701604,0.00030326055,0.0036000255,0.006031784],"study_design_scores_gemma":[0.0000015059524,0.000011004127,0.9991135,0.0000037743555,0.00000604674,0.00008546749,0.000056219098,0.000086835105,0.000090668625,0.0000653966,0.0004774378,0.0000020991092],"about_ca_topic_score_codex":0.01853584,"about_ca_topic_score_gemma":0.019835941,"teacher_disagreement_score":0.01853584,"about_ca_system_score_codex":0.0005302469,"about_ca_system_score_gemma":0.00020150232,"threshold_uncertainty_score":0.036855936},"labels":[],"label_agreement":null},{"id":"W1987541937","doi":"10.1088/0004-637x/767/1/93","title":"HALO ORBITS IN COSMOLOGICAL DISK GALAXIES: TRACERS OF FORMATION HISTORY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Halo; Stars; Galactic halo; Galaxy; Metallicity; Dark matter halo; Bulge; Orbit (dynamics); Milky Way","score_opus":0.017001845091702585,"score_gpt":0.2394279403806331,"score_spread":0.2224260952889305,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987541937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990872,0.00005183863,0.0004594115,0.00001817617,7.7496526e-7,0.0000024741132,0.000096040574,0.000029166515,0.00025481117],"genre_scores_gemma":[0.99889106,0.00003347311,0.0007715254,0.0000042230463,0.000001600424,0.0000027860985,0.00019846039,0.000013166204,0.00008372832],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999293,0.00002870996,0.0000032906667,0.000011570958,0.000014577429,0.000012481205],"domain_scores_gemma":[0.999047,0.00033686846,0.00021147783,0.00009975207,0.00006538295,0.00023946627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047422014,0.00019210528,0.0001950529,0.0013758177,0.0002673951,0.00044321382,0.00037175027,0.00029474546,0.0005095211],"category_scores_gemma":[0.0024052947,0.00019048904,0.00028112024,0.0010023786,0.00035846554,0.00033367457,0.00058146095,0.00025169863,0.00008705921],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041482318,0.00010773603,0.72368926,0.00004711628,0.00028921512,0.0003010745,0.0009962918,0.25254738,0.01033213,0.0034107638,0.0004545634,0.0074097454],"study_design_scores_gemma":[0.00006526345,0.00014119832,0.39235148,0.000017309048,0.000054597876,0.00014240663,0.00037101068,0.59976286,0.0027324439,0.0030313125,0.0012915579,0.000038609942],"about_ca_topic_score_codex":0.011989854,"about_ca_topic_score_gemma":0.010377888,"teacher_disagreement_score":0.011989854,"about_ca_system_score_codex":0.0007253236,"about_ca_system_score_gemma":0.00021463075,"threshold_uncertainty_score":0.02384013},"labels":[],"label_agreement":null},{"id":"W1987577604","doi":"10.1088/0004-637x/799/1/43","title":"THE STRUCTURE OF PRE-TRANSITIONAL PROTOPLANETARY DISKS. II. AZIMUTHAL ASYMMETRIES, DIFFERENT RADIAL DISTRIBUTIONS OF LARGE AND SMALL DUST GRAINS IN PDS 70<sup>,</sup>","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Smithsonian Astrophysical Observatory; National Astronomical Observatory of Japan; Academia Sinica; Japan Society for the Promotion of Science; Ministry of Education, Culture, Sports, Science and Technology; Smithsonian Institution; National Science Foundation","keywords":"Physics; Protoplanetary disk; Astrophysics; Debris disk; Millimeter; Photoevaporation; RADIUS; Wavelength; Thick disk; Position angle; T Tauri star; Protoplanet; Astronomy; Planet; Planetary system; Stars; Optics; Galaxy; Halo","score_opus":0.010248137433261783,"score_gpt":0.22991287836529833,"score_spread":0.21966474093203656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987577604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978338,0.00042092774,0.00023319288,0.000033175093,0.0000025138002,0.0000041365006,0.00022306663,0.000020726851,0.001228358],"genre_scores_gemma":[0.9992067,0.00010063214,0.00020432235,0.000017576527,0.000003860984,0.000003144273,0.00031195217,0.000003649153,0.00014823869],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996364,0.0000019158701,0.0000021471424,0.000012449274,0.0000084391595,0.000011342276],"domain_scores_gemma":[0.9999205,0.000005469231,0.000034077235,0.000005205813,0.000011084158,0.000023639124],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000031382242,0.00016823228,0.00009578476,0.00043061867,0.00030074592,0.00035318732,0.00022965006,0.0002631909,0.0005999471],"category_scores_gemma":[0.00010972181,0.0001484756,0.0001075824,0.0002581265,0.00027004498,0.00021554047,0.00029685828,0.00022665059,0.00019918787],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005361693,0.000041734267,0.3802141,0.00015766338,0.000049729122,0.0014092169,0.00067367585,0.0007544368,0.5977213,0.0008304272,0.00070208905,0.016909564],"study_design_scores_gemma":[0.0000061793608,0.000041419164,0.988091,0.000004911698,0.000011742011,0.0008983312,0.000356936,0.0005828365,0.008914186,0.00022920556,0.00085961225,0.000003691632],"about_ca_topic_score_codex":0.0019024387,"about_ca_topic_score_gemma":0.0028312074,"teacher_disagreement_score":0.0019024387,"about_ca_system_score_codex":0.00032971738,"about_ca_system_score_gemma":0.00009966652,"threshold_uncertainty_score":0.0037827492},"labels":[],"label_agreement":null},{"id":"W1987579510","doi":"10.1086/590531","title":"Measurements of Energy Partitioning in H <sub>2</sub> Formation by Photolysis of Amorphous Water Ice","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Photodissociation; Endothermic process; Exothermic reaction; Amorphous ice; Amorphous solid; Physics; Hydrogen atom; Molecule; Atomic physics; Atom (system on chip); Chemical physics; Hydrogen; Astrochemistry; Water ice; Hydrogen atom abstraction; Photochemistry; Hydrogen molecule; Molecular physics; Physical chemistry; Astrophysics; Interstellar medium; Chemistry; Astrobiology; Crystallography; Thermodynamics; Adsorption","score_opus":0.015728233021079528,"score_gpt":0.20706582250184488,"score_spread":0.19133758948076535,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987579510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99699736,0.00014160729,0.0019835136,0.000017077706,0.0000023007217,0.000009450399,0.000069100824,0.000018746603,0.00076104514],"genre_scores_gemma":[0.99928564,0.0000576245,0.00041092647,0.000006179274,0.000001138171,0.000007926442,0.00004292794,0.0000064928845,0.00018102488],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999298,0.0000073158744,0.0000018818255,0.000021934722,0.000021333588,0.000017708933],"domain_scores_gemma":[0.99986434,0.00006405651,0.00003286415,0.000009794852,0.000016096365,0.000012747537],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008145312,0.00019614468,0.00012483512,0.0002165199,0.00027711925,0.00020487283,0.00022596464,0.00023125672,0.0011742387],"category_scores_gemma":[0.0002542606,0.00015877438,0.00008453361,0.00017723133,0.00043371582,0.00038675207,0.00027023634,0.0003913741,0.00016201923],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016654807,0.000019798517,0.0033274768,0.00002599802,0.000009198566,0.000044999873,0.00009180657,0.00043400796,0.9936604,0.00025090753,0.000024586607,0.0019441845],"study_design_scores_gemma":[0.000016659931,0.00013960408,0.022170968,0.0000034177617,0.0000087719445,0.00009391964,0.0001331314,0.0031403732,0.97341317,0.0003225809,0.0005498795,0.000007462608],"about_ca_topic_score_codex":0.0006372626,"about_ca_topic_score_gemma":0.0005728629,"teacher_disagreement_score":0.0011742387,"about_ca_system_score_codex":0.00029348137,"about_ca_system_score_gemma":0.000081439684,"threshold_uncertainty_score":0.003928244},"labels":[],"label_agreement":null},{"id":"W1987593507","doi":"10.1088/0004-637x/703/1/399","title":"AN INFRARED/X-RAY SURVEY FOR NEW MEMBERS OF THE TAURUS STAR-FORMING REGION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":192,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Stars; Brown dwarf; Stellar classification; Initial mass function; Spitzer Space Telescope; Molecular cloud; Spectral line; Low Mass","score_opus":0.021449847454829044,"score_gpt":0.26520315717228554,"score_spread":0.2437533097174565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987593507","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989593,0.00023464115,0.0001477473,0.000043096054,0.0000033864649,0.000010442751,0.00009407417,0.000011561696,0.00049579045],"genre_scores_gemma":[0.99674773,0.0003032717,0.0012323118,0.00008739456,0.00006823545,0.000014338544,0.00083273626,0.0000069488533,0.000707138],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997639,0.000028396364,0.000020689415,0.000051527953,0.000092595306,0.00004282856],"domain_scores_gemma":[0.9989278,0.00013108058,0.00037005806,0.00007796538,0.00016470285,0.00032830978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005993747,0.0002508278,0.00020570475,0.0018513456,0.00066629954,0.0005076404,0.00030979162,0.0002972531,0.0014626302],"category_scores_gemma":[0.00064095383,0.00016305063,0.0002113152,0.00069932285,0.00020875984,0.0005718322,0.00040450017,0.00031653378,0.0004341744],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006299991,0.00015724037,0.9739899,0.000022008755,0.00003528627,0.00034228835,0.0006262212,0.000045886245,0.010909849,0.000046132485,0.00028470598,0.0134774605],"study_design_scores_gemma":[0.0000059195945,0.00015138538,0.99634016,0.000005811663,0.00002022391,0.0007542795,0.00017053944,0.00012246768,0.0008202163,0.000020428082,0.0015850497,0.0000034929037],"about_ca_topic_score_codex":0.0014503925,"about_ca_topic_score_gemma":0.003159546,"teacher_disagreement_score":0.0018513456,"about_ca_system_score_codex":0.00016512464,"about_ca_system_score_gemma":0.0001870103,"threshold_uncertainty_score":0.004893005},"labels":[],"label_agreement":null},{"id":"W1987633527","doi":"10.1088/0004-637x/796/1/65","title":"THE PHASE SPACE AND STELLAR POPULATIONS OF CLUSTER GALAXIES AT<i>z</i>∼ 1: SIMULTANEOUS CONSTRAINTS ON THE LOCATION AND TIMESCALE OF SATELLITE QUENCHING","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Quenching (fluorescence); Galaxy; Redshift; Population; Satellite galaxy; Cluster (spacecraft); Galaxy cluster; Phase (matter)","score_opus":0.00829674347102467,"score_gpt":0.22573126706872632,"score_spread":0.21743452359770166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987633527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953973,0.000013236854,0.00024405429,0.000010518194,2.7896297e-7,0.0000016980165,0.00005196771,0.0000074103677,0.00013114288],"genre_scores_gemma":[0.99968266,0.000011318939,0.00014673655,0.000002532026,7.930153e-7,0.000001912477,0.00012609037,0.000003128162,0.00002475032],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999416,0.000009366791,0.0000020207829,0.000020619771,0.000007193737,0.000019247178],"domain_scores_gemma":[0.99941385,0.00021984929,0.00018011968,0.000056355137,0.000034094417,0.0000957334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030241872,0.00016307473,0.00021960239,0.0004179444,0.0002690358,0.0005230592,0.0004632635,0.00029333256,0.0008278046],"category_scores_gemma":[0.0014397927,0.00021116534,0.00034027704,0.0004327379,0.00038112764,0.00039585566,0.00034850655,0.00024853158,0.0000894304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003409786,0.000063723266,0.81541413,0.000030074427,0.0001317872,0.000104415834,0.00043973164,0.15448089,0.018101014,0.003316666,0.00027436326,0.007302127],"study_design_scores_gemma":[0.00006885429,0.00012336664,0.6858712,0.000009780454,0.000060389757,0.00006999391,0.00017210956,0.30907044,0.0022014712,0.0018566025,0.0004671201,0.000028715775],"about_ca_topic_score_codex":0.02027596,"about_ca_topic_score_gemma":0.02018811,"teacher_disagreement_score":0.02027596,"about_ca_system_score_codex":0.0007976625,"about_ca_system_score_gemma":0.0002831052,"threshold_uncertainty_score":0.040315866},"labels":[],"label_agreement":null},{"id":"W1987705592","doi":"10.1088/0004-637x/703/2/2068","title":"WARPS AND BARS FROM THE EXTERNAL TIDAL TORQUES OF TUMBLING DARK HALOS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Dark matter; Galaxy; Halo; Spiral galaxy; Dark matter halo; Cold dark matter; Tidal force","score_opus":0.007122893186335841,"score_gpt":0.2126223054964358,"score_spread":0.20549941231009994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987705592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964935,0.000033707347,0.0014254322,0.00008145996,0.000012953407,0.000007049526,0.0000559238,0.00007350982,0.0018164816],"genre_scores_gemma":[0.99936336,0.000018758468,0.00028157368,0.000015119831,0.0000029582886,0.0000033910542,0.000036806967,0.00001989446,0.00025811882],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999912,0.000019926578,0.0000047514063,0.000012675046,0.000022162601,0.00002844923],"domain_scores_gemma":[0.9994054,0.00018590628,0.000106330335,0.00008674093,0.000051809162,0.00016391392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032641928,0.00033282756,0.0002768214,0.00040457194,0.0003757232,0.00059175206,0.0003077305,0.0003477104,0.0019407027],"category_scores_gemma":[0.0019114199,0.00026645424,0.0003217999,0.00020418872,0.00066035683,0.0004206476,0.0007919212,0.00045966203,0.00014441731],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010121249,0.00025024175,0.055873703,0.00019502825,0.00023161549,0.001584818,0.00068465574,0.78507525,0.1261377,0.008696178,0.0018305352,0.018428227],"study_design_scores_gemma":[0.0001529163,0.00029460044,0.054511704,0.000028600922,0.000062222345,0.00020316528,0.00025844216,0.918577,0.020345408,0.00439757,0.0011205614,0.000047815065],"about_ca_topic_score_codex":0.0026293208,"about_ca_topic_score_gemma":0.0031825758,"teacher_disagreement_score":0.0026293208,"about_ca_system_score_codex":0.00042240438,"about_ca_system_score_gemma":0.00019553445,"threshold_uncertainty_score":0.006492257},"labels":[],"label_agreement":null},{"id":"W1987716798","doi":"10.1086/318896","title":"A New Radio–X-Ray Probe of Galaxy Cluster Magnetic Fields","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":542,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; ROSAT; Physics; Cluster (spacecraft); Galaxy cluster; Redshift; Luminosity; Magnetic field; Faraday effect; Cooling flow; Galaxy; Astronomy","score_opus":0.006247375393840545,"score_gpt":0.20283223645982326,"score_spread":0.19658486106598272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987716798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9804638,0.0012504935,0.008759158,0.00022273479,0.000033518423,0.000039575152,0.0016271719,0.00020625371,0.007397255],"genre_scores_gemma":[0.9769857,0.00037619242,0.014991657,0.00023273868,0.000082687315,0.000078536155,0.0032445919,0.000049030572,0.0039589503],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998234,0.000022715214,0.0000060141933,0.000058021487,0.00004477699,0.00004518063],"domain_scores_gemma":[0.99944776,0.000079569756,0.00016381414,0.00008455887,0.00009327236,0.00013093713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036582758,0.00019780474,0.00024628756,0.001056254,0.00033432068,0.00062698935,0.0004608883,0.00034016964,0.002499249],"category_scores_gemma":[0.00040222576,0.00022595409,0.0002440794,0.0007463273,0.00035141665,0.0005147888,0.0006750713,0.00045739356,0.00051931775],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011113674,0.000546021,0.3874425,0.00024548787,0.00039570965,0.0005271594,0.00040040354,0.0015317744,0.5434462,0.0016224349,0.003553877,0.059177097],"study_design_scores_gemma":[0.00007016038,0.00035762414,0.9620365,0.000014275957,0.00011717111,0.0012093659,0.00014607862,0.0029581839,0.021204066,0.00065998104,0.0111831175,0.000043439773],"about_ca_topic_score_codex":0.001601658,"about_ca_topic_score_gemma":0.0045443834,"teacher_disagreement_score":0.002499249,"about_ca_system_score_codex":0.00034142195,"about_ca_system_score_gemma":0.0001293144,"threshold_uncertainty_score":0.008360803},"labels":[],"label_agreement":null},{"id":"W1987769530","doi":"10.1086/422408","title":"Observations of PSR J2021+3651 and its X‐Ray Pulsar Wind Nebula G75.2+0.1","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Nebula; Vela; Millisecond pulsar; Torus; Telescope; Flux (metallurgy); Emission nebula; Pulsar wind nebula","score_opus":0.022765356310919034,"score_gpt":0.3101420710558898,"score_spread":0.2873767147449708,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987769530","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99903333,0.00009148455,0.00005003454,0.000010136876,0.0000029158196,0.0000057548586,0.00028035173,0.000022712877,0.0005034195],"genre_scores_gemma":[0.99797755,0.000092479844,0.00029853205,0.00001898357,0.000006296238,0.0000048451398,0.0013048953,0.000005920807,0.00029048906],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999417,0.0000029577318,0.0000030394592,0.000016529219,0.000015277641,0.000020566667],"domain_scores_gemma":[0.999892,0.0000055390756,0.000033325836,0.000009463756,0.0000061028463,0.000053557214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000953148,0.00033300914,0.00021878521,0.00057810004,0.00042042852,0.00034715582,0.00020380593,0.00021432748,0.00047068816],"category_scores_gemma":[0.00014731246,0.00012359311,0.00015144718,0.0005453252,0.0001589804,0.00013581834,0.0003639929,0.00016515896,0.00016784517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018091488,0.00042306198,0.5540208,0.00021261029,0.00027294803,0.005717035,0.0014117716,0.003625752,0.39378458,0.0009398357,0.0020362807,0.03574622],"study_design_scores_gemma":[0.000026671876,0.0002117756,0.9906962,0.0000059514587,0.000035360885,0.0007209835,0.00011807709,0.00079128385,0.0041733515,0.000080504156,0.0031278965,0.000011941331],"about_ca_topic_score_codex":0.008880962,"about_ca_topic_score_gemma":0.013500029,"teacher_disagreement_score":0.008880962,"about_ca_system_score_codex":0.00035453826,"about_ca_system_score_gemma":0.00017666545,"threshold_uncertainty_score":0.017658532},"labels":[],"label_agreement":null},{"id":"W1987784068","doi":"10.1088/0004-637x/697/2/1971","title":"HISTORY OF GALAXY INTERACTIONS AND THEIR IMPACT ON STAR FORMATION OVER THE LAST 7 Gyr FROM GEMS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":241,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Natural Science Foundation of China; Space Telescope Science Institute; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; Johns Hopkins University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Astrophysics; Physics; Galaxy; Halo; Star formation; Minor (academic); Galaxy formation and evolution; Stellar mass; Mass fraction; Galaxy merger; Astronomy; Humanities; Art; Thermodynamics","score_opus":0.00795236591899986,"score_gpt":0.2159308857355548,"score_spread":0.20797851981655494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987784068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979674,0.00019008349,0.00007133564,0.000035189118,0.0000028698244,0.0000012237861,0.0010583485,0.000014711681,0.0006587542],"genre_scores_gemma":[0.9975823,0.000085816224,0.00007653083,0.000008205631,0.000007533129,0.0000010360644,0.00192963,0.0000049721143,0.0003040016],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997924,0.000026601503,0.000013971987,0.000055034398,0.00005182789,0.000060223836],"domain_scores_gemma":[0.9985159,0.00023660902,0.00063610554,0.00012311153,0.00018931158,0.00029903624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004084804,0.00018433863,0.0001995871,0.0009129042,0.0002841612,0.0007020018,0.000251678,0.00021883739,0.0014405615],"category_scores_gemma":[0.0018713671,0.000110965724,0.0002914623,0.00070537295,0.00020426234,0.0004499354,0.0007336736,0.000309986,0.00047455743],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004211888,0.000011287565,0.9947208,0.0000067978885,0.000039558763,0.000077847144,0.0001281077,0.00035486344,0.0007218126,0.000067890745,0.0002434363,0.003585505],"study_design_scores_gemma":[4.341633e-7,0.000011409138,0.99897444,0.0000017137593,0.000006427741,0.000042451986,0.000041235406,0.00033854635,0.00011823265,0.000015233533,0.0004486538,0.0000013445781],"about_ca_topic_score_codex":0.0088121705,"about_ca_topic_score_gemma":0.012818722,"teacher_disagreement_score":0.0088121705,"about_ca_system_score_codex":0.0003415916,"about_ca_system_score_gemma":0.00015132767,"threshold_uncertainty_score":0.017521739},"labels":[],"label_agreement":null},{"id":"W1987844855","doi":"10.1086/424727","title":"Simultaneous Production of Disk and Lobes: A Single‐Wind MHD Model for the η Carinae Nebula","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Magnetohydrodynamics; Stellar rotation; Bipolar outflow; Nebula; Planetary nebula; Rotation (mathematics); Magnetohydrodynamic drive; Magnetic field; Astronomy; Stars; Star formation; Geometry","score_opus":0.014028190075120822,"score_gpt":0.22499559722824725,"score_spread":0.21096740715312642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987844855","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9334093,0.0015288693,0.026391791,0.001894118,0.0001967246,0.00017449906,0.00088633737,0.00027123693,0.03524721],"genre_scores_gemma":[0.99222046,0.0003864292,0.0025002337,0.00010251586,0.00007117176,0.00009093288,0.00017181544,0.00003915647,0.0044171433],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992216,0.000019136458,0.000004698002,0.000017193823,0.000015346573,0.00002145912],"domain_scores_gemma":[0.9997986,0.000039283124,0.000032946657,0.000013580623,0.00002586279,0.0000897862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019694093,0.00063241617,0.00066429627,0.0003905091,0.0010088932,0.0014329453,0.0014431545,0.0025296407,0.001878978],"category_scores_gemma":[0.0005469298,0.00052315625,0.0009918243,0.00029530883,0.0010591173,0.0008140559,0.0012558647,0.0006673253,0.00052303134],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036031377,0.00017308319,0.0074520353,0.00008263815,0.0000749467,0.001347443,0.00032456408,0.9618394,0.008161346,0.016532227,0.0010571583,0.0025947823],"study_design_scores_gemma":[0.00015365369,0.0000698944,0.0014553698,0.0000070236874,0.000015634414,0.00007632948,0.000055239787,0.9952186,0.00015709046,0.00220064,0.00056956423,0.000020836535],"about_ca_topic_score_codex":0.017772298,"about_ca_topic_score_gemma":0.0044775275,"teacher_disagreement_score":0.017772298,"about_ca_system_score_codex":0.0010290507,"about_ca_system_score_gemma":0.0006946579,"threshold_uncertainty_score":0.035337687},"labels":[],"label_agreement":null},{"id":"W1987845920","doi":"10.1086/462408","title":"First Results from the Canada‐France High‐<i>z</i>Quasar Survey: Constraints on the<i>z</i>= 6 Quasar Luminosity Function and the Quasar Contribution to Reionization","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Reionization; Physics; Luminosity function; Astrophysics; OVV quasar; Luminosity; Astronomy; Redshift; Function (biology); Galaxy","score_opus":0.008837198199238916,"score_gpt":0.19471980911944883,"score_spread":0.1858826109202099,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987845920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89273506,0.003373802,0.0035656635,0.0031061587,0.00010994197,0.0002233906,0.04217152,0.0003983365,0.05431614],"genre_scores_gemma":[0.9346277,0.0014923651,0.0038036513,0.0015723933,0.000101790305,0.00012894624,0.025976248,0.0001804685,0.032116365],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989503,0.00011008002,0.000022755628,0.000113306254,0.00039918162,0.0004044236],"domain_scores_gemma":[0.9972326,0.00025641118,0.00026983782,0.00018068227,0.0014215542,0.0006388337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011282198,0.00072506064,0.0005540969,0.0021252676,0.0020023002,0.0018528795,0.00062200817,0.0008586384,0.0033435202],"category_scores_gemma":[0.0015897827,0.00030078206,0.0007903516,0.0026379416,0.00061657804,0.00031674115,0.0012575921,0.0005412803,0.0010295802],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00095262035,0.0002274248,0.8748464,0.00022426473,0.0005683454,0.00071689195,0.0019057015,0.0032264525,0.013478093,0.0034073777,0.042499512,0.057946857],"study_design_scores_gemma":[0.00003302747,0.000038602346,0.97395575,0.000021637254,0.00007693623,0.0000869137,0.0005171598,0.00026847213,0.0011636168,0.00013482373,0.023674684,0.00002839166],"about_ca_topic_score_codex":0.9411982,"about_ca_topic_score_gemma":0.9761571,"teacher_disagreement_score":0.9411982,"about_ca_system_score_codex":0.009682819,"about_ca_system_score_gemma":0.0100160055,"threshold_uncertainty_score":0.11829609},"labels":[],"label_agreement":null},{"id":"W1987860029","doi":"10.1086/587136","title":"AEGIS: Radio and Mid‐Infrared Selection of Obscured AGN Candidates","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Active galactic nucleus; Astrophysics; Observatory; Physics; Infrared; Spitzer Space Telescope; Telescope; Mid infrared; Selection (genetic algorithm); Astronomy; Wavelength; Galaxy; Computer science; Optics; Artificial intelligence","score_opus":0.006669499256835492,"score_gpt":0.1958863110660864,"score_spread":0.1892168118092509,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987860029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900339,0.00028800842,0.00159732,0.000066882494,0.000014535582,0.000069766334,0.002680414,0.0001340768,0.005115157],"genre_scores_gemma":[0.98188937,0.0002996434,0.007896229,0.00009610692,0.000039382703,0.00005520952,0.0065226345,0.000040021587,0.0031614127],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983287,0.00002893331,0.000015583273,0.000036890233,0.00004168654,0.000043978143],"domain_scores_gemma":[0.999577,0.000058963953,0.00014046987,0.000057700094,0.00006215487,0.000103637845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049016374,0.0002547452,0.00027817494,0.0015906972,0.00027923755,0.00045842302,0.00020511013,0.00012557617,0.002251209],"category_scores_gemma":[0.0007980482,0.000106904285,0.00016835134,0.00054743595,0.000093125156,0.00022950975,0.0004387391,0.00014578916,0.00068991195],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000509143,0.000098371376,0.89041245,0.0000690126,0.000093211944,0.0004590775,0.00020269601,0.0006309078,0.04545119,0.000639005,0.004912604,0.05652229],"study_design_scores_gemma":[0.000024893507,0.00008517928,0.9859378,0.000010089175,0.000045130775,0.000709563,0.00014886985,0.0026563585,0.00464286,0.00016992848,0.0055602374,0.000009122358],"about_ca_topic_score_codex":0.0030728693,"about_ca_topic_score_gemma":0.009636687,"teacher_disagreement_score":0.0030728693,"about_ca_system_score_codex":0.00017014085,"about_ca_system_score_gemma":0.00016479463,"threshold_uncertainty_score":0.007531047},"labels":[],"label_agreement":null},{"id":"W1987965478","doi":"10.1088/0004-637x/765/2/158","title":"A METAL-RICH LOW-GRAVITY COMPANION TO A MASSIVE MILLISECOND PULSAR","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Millisecond pulsar; White dwarf; Pulsar; Binary pulsar; Binary number; Solar mass; Roche lobe; Neutron star; Binary star","score_opus":0.010371986332161357,"score_gpt":0.2909235267015115,"score_spread":0.28055154036935015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987965478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99872226,0.00009639743,0.0001941287,0.000041599986,0.000009421393,0.0000030489132,0.000041331517,0.000018894349,0.0008728759],"genre_scores_gemma":[0.99882907,0.000047836522,0.00029363652,0.000032041367,0.00001269464,0.0000015191313,0.00015628402,0.000002335426,0.00062453275],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999441,0.0000034060122,0.000005272287,0.000019509203,0.000011627456,0.000016037857],"domain_scores_gemma":[0.9998386,0.000014634524,0.00005101773,0.000015011562,0.000008260459,0.00007249608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009254716,0.00016089692,0.00019431577,0.00029674682,0.00053276576,0.00058700814,0.0002430555,0.00030338415,0.0012624731],"category_scores_gemma":[0.00035628624,0.00012423981,0.00011552055,0.00024099853,0.00020725689,0.0002327057,0.00054537045,0.00026978352,0.0005141674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004681688,0.00024193781,0.7998529,0.000090365735,0.00004474644,0.016933676,0.0009093155,0.00040645566,0.15617433,0.0015472942,0.0011500291,0.02218072],"study_design_scores_gemma":[0.000068153255,0.0012093398,0.9190927,0.00002220927,0.000049106697,0.040386524,0.00056598167,0.0020154598,0.02174755,0.0013283571,0.01349611,0.000018427309],"about_ca_topic_score_codex":0.0009962384,"about_ca_topic_score_gemma":0.0012871596,"teacher_disagreement_score":0.0012624731,"about_ca_system_score_codex":0.00022705938,"about_ca_system_score_gemma":0.0001455755,"threshold_uncertainty_score":0.004223466},"labels":[],"label_agreement":null},{"id":"W1987985136","doi":"10.1086/498666","title":"The Boomerang PWN G106.6+2.9 and the Magnetic Field Structure in Pulsar Wind Nebulae","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Pulsar; Pulsar wind nebula; Astrophysics; Supernova remnant; Nebula; Supernova; Astronomy; Magnetic field; Magnetar; Galactic plane; Galaxy; Stars","score_opus":0.0030935014183804985,"score_gpt":0.25440400959137593,"score_spread":0.25131050817299544,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1987985136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98593444,0.0005385542,0.00009579342,0.00080320676,0.000121434234,0.00000892089,0.0002995414,0.00001607493,0.012182067],"genre_scores_gemma":[0.9930774,0.00028260826,0.00007723214,0.0001554481,0.00013427225,0.0000034542638,0.00056708005,0.000023438914,0.0056791403],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999311,0.000012347068,0.0000032660298,0.000018903746,0.00001691421,0.000017448028],"domain_scores_gemma":[0.9996119,0.00004479784,0.00011718094,0.000020450785,0.000082837694,0.0001229344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023448367,0.00016819379,0.00022413836,0.0005351025,0.0006606348,0.00089064805,0.00017827147,0.00038723703,0.0068423063],"category_scores_gemma":[0.000752252,0.00010695026,0.00005644117,0.0006302873,0.00041244115,0.0002564205,0.00041717617,0.0003011637,0.0014783948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016934888,0.00029904398,0.80919695,0.00033944697,0.00015298894,0.0034872312,0.0017884555,0.0010076055,0.055147514,0.010730283,0.028152635,0.08800441],"study_design_scores_gemma":[0.00004631496,0.00009879017,0.9785841,0.000025384725,0.000021634762,0.00071587117,0.00029337968,0.0002468877,0.00095485995,0.0016280051,0.017374747,0.000009890155],"about_ca_topic_score_codex":0.00238947,"about_ca_topic_score_gemma":0.0040292577,"teacher_disagreement_score":0.0068423063,"about_ca_system_score_codex":0.00020433597,"about_ca_system_score_gemma":0.00019183147,"threshold_uncertainty_score":0.022889853},"labels":[],"label_agreement":null},{"id":"W1988001480","doi":"10.1088/0004-637x/761/1/66","title":"POST-OUTBURST X-RAY FLUX AND TIMING EVOLUTION OF SWIFT J1822.3–1606","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Swift; Astrophysics; Physics; Flux (metallurgy); Light curve; Static timing analysis; Telescope; Noise (video); Exponential decay; Pulsar; Nuclear physics","score_opus":0.012838946116034438,"score_gpt":0.23109822936751934,"score_spread":0.2182592832514849,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988001480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988937,0.00005025694,0.000102756225,0.000020863297,0.0000052220953,0.0000034874581,0.00045412214,0.000020504203,0.0004489899],"genre_scores_gemma":[0.997517,0.000056789926,0.00024050186,0.000014330806,0.000016570288,0.00000708292,0.0017243699,0.00002476909,0.000398645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.0000062483596,0.0000062171894,0.00002686447,0.000020891584,0.000022758673],"domain_scores_gemma":[0.9993247,0.00005926564,0.000297656,0.000037017242,0.00012691005,0.00015452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018066666,0.00029551444,0.00030198367,0.0011531931,0.00024151494,0.00045753483,0.00022589313,0.00026903325,0.0008142153],"category_scores_gemma":[0.0008317782,0.00016149867,0.0002514106,0.00067777856,0.00014911036,0.00021246354,0.0002409289,0.00029630214,0.00032240947],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034319118,0.00019382573,0.90804297,0.000059422913,0.00009532793,0.0011889623,0.0004102872,0.0019006693,0.07429744,0.0002945352,0.0009723624,0.012200939],"study_design_scores_gemma":[0.0000023554867,0.000023541495,0.997908,0.0000026014445,0.0000063871116,0.00013597196,0.00002126805,0.00087018154,0.0007242179,0.000016147924,0.00028535008,0.000004008737],"about_ca_topic_score_codex":0.00518797,"about_ca_topic_score_gemma":0.0075650127,"teacher_disagreement_score":0.00518797,"about_ca_system_score_codex":0.00028712003,"about_ca_system_score_gemma":0.00010543741,"threshold_uncertainty_score":0.010315537},"labels":[],"label_agreement":null},{"id":"W1988078506","doi":"10.1086/346078","title":"The Optical Design and Characterization of the<i>Microwave Anisotropy Probe</i>","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Cosmic microwave background; Sky; Microwave; Physics; Ranging; Radiometer; Remote sensing; Optics; Offset (computer science); Microwave radiometer; Anisotropy; Polarization (electrochemistry); Satellite; Astronomy; Astrophysics; Computer science; Geology; Geodesy","score_opus":0.008579720091921126,"score_gpt":0.19794174788084823,"score_spread":0.1893620277889271,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988078506","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.41433147,0.00048396474,0.5535125,0.00097378576,0.00015138446,0.00077806663,0.0020233411,0.0024321808,0.025313318],"genre_scores_gemma":[0.6031959,0.00019294515,0.3907158,0.00039414447,0.00010247797,0.00057189795,0.00093134923,0.00010693996,0.00378853],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99962103,0.00006655672,0.000011345778,0.00009255056,0.00013318995,0.000075328004],"domain_scores_gemma":[0.999241,0.000111998066,0.00018825695,0.0001778608,0.0002174722,0.00006348121],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006508571,0.00042082305,0.00016208862,0.00044103028,0.0005782866,0.00089338137,0.0008089531,0.00054928515,0.0012752041],"category_scores_gemma":[0.001167703,0.00030358435,0.00016420534,0.0004978366,0.0006004743,0.0005949498,0.00057218596,0.00042091534,0.0006313987],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006052513,0.000222561,0.048507035,0.00034156055,0.00005666379,0.00017518764,0.00037752543,0.011696353,0.7119641,0.03750664,0.004736867,0.1838103],"study_design_scores_gemma":[0.00012705915,0.0007875694,0.042824786,0.000037750222,0.000097396114,0.00077401503,0.00014950823,0.04324409,0.83320284,0.004189111,0.07447235,0.000093479764],"about_ca_topic_score_codex":0.002132012,"about_ca_topic_score_gemma":0.0032989883,"teacher_disagreement_score":0.002132012,"about_ca_system_score_codex":0.00078961236,"about_ca_system_score_gemma":0.00082534284,"threshold_uncertainty_score":0.0057290792},"labels":[],"label_agreement":null},{"id":"W1988112885","doi":"10.1088/0004-637x/780/2/138","title":"SIMPLE ANALYTICAL FORMS OF THE PERPENDICULAR DIFFUSION COEFFICIENT FOR TWO-COMPONENT TURBULENCE. II. DYNAMICAL TURBULENCE WITH CONSTANT CORRELATION TIME","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Turbulence; Constant (computer programming); Diffusion; Simple (philosophy); K-epsilon turbulence model; Component (thermodynamics); K-omega turbulence model; Statistical physics; Classical mechanics; Mechanics; Thermodynamics","score_opus":0.003580749756000276,"score_gpt":0.20597488450206727,"score_spread":0.202394134746067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988112885","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.09251789,0.0052946424,0.7818344,0.0020459977,0.0007483213,0.00029205723,0.0011503454,0.00076185755,0.11535446],"genre_scores_gemma":[0.8745297,0.0044579874,0.07453504,0.00050726696,0.0003617139,0.00025269345,0.00064971764,0.0003183981,0.044387493],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998858,0.000014612065,0.00000978287,0.000026108013,0.000040451923,0.000023329447],"domain_scores_gemma":[0.99974173,0.00006600953,0.00007217368,0.000033134053,0.000060321432,0.000026604695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023576552,0.0006747446,0.0002835393,0.00077314506,0.00031151678,0.0008660689,0.0006297484,0.00082095584,0.0046229768],"category_scores_gemma":[0.0014199323,0.00017542747,0.00039850452,0.00052222185,0.0007490392,0.0015205004,0.0005661314,0.0009159824,0.0010782506],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040426326,0.00006307518,0.00097261,0.00032262984,0.00001689354,0.00045949724,0.00021816387,0.048724554,0.04113947,0.87961954,0.0074450737,0.02097791],"study_design_scores_gemma":[0.000022424192,0.00003118128,0.0022154828,0.00008004751,0.000017533299,0.0008320374,0.000116475116,0.65607864,0.007291319,0.31643185,0.016783793,0.00009922034],"about_ca_topic_score_codex":0.0013814232,"about_ca_topic_score_gemma":0.0013253689,"teacher_disagreement_score":0.0046229768,"about_ca_system_score_codex":0.0005536067,"about_ca_system_score_gemma":0.00048712618,"threshold_uncertainty_score":0.015465379},"labels":[],"label_agreement":null},{"id":"W1988119723","doi":"10.1088/0004-637x/696/2/1755","title":"SPECTROSCOPIC ANALYSIS OF DA WHITE DWARFS: STARK BROADENING OF HYDROGEN LINES INCLUDING NONIDEAL EFFECTS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":375,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Stark effect; White dwarf; Physics; Spectral line; Line (geometry); Atomic physics; Ideal (ethics); Computational physics; Electron; Stars; Quantum mechanics; Astrophysics; Law","score_opus":0.010039848906097285,"score_gpt":0.2528303456615756,"score_spread":0.2427904967554783,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988119723","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90129066,0.00026351566,0.0925453,0.00010867368,0.000018811315,0.000022612405,0.00017752041,0.0005211722,0.005051733],"genre_scores_gemma":[0.989518,0.00007745969,0.009345134,0.000022193632,0.000013596486,0.000011947633,0.00010820465,0.00004121802,0.0008623356],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99990857,0.000019459343,0.0000044621856,0.000017983655,0.00003580152,0.000013842025],"domain_scores_gemma":[0.9996991,0.00005635864,0.000057458048,0.000077155324,0.000066372384,0.000043613134],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028435196,0.0004718301,0.00034937996,0.0004133242,0.00036720707,0.00040857852,0.00091769325,0.00045394755,0.00052572764],"category_scores_gemma":[0.0008211077,0.00021556679,0.00041955648,0.000322885,0.00023550467,0.0004233075,0.00051247573,0.00026559265,0.00018175157],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000109743334,0.000098798344,0.061960492,0.000087111606,0.00009210476,0.00047977094,0.0002494991,0.87358713,0.0356135,0.009334706,0.0006732899,0.017713899],"study_design_scores_gemma":[0.00001951869,0.00003837929,0.012862382,0.0000026202008,0.0000148170375,0.000078633995,0.000028774712,0.9786861,0.0048985234,0.002407394,0.000950269,0.000012655856],"about_ca_topic_score_codex":0.007197453,"about_ca_topic_score_gemma":0.0059280987,"teacher_disagreement_score":0.007197453,"about_ca_system_score_codex":0.00057777227,"about_ca_system_score_gemma":0.00032091388,"threshold_uncertainty_score":0.014311075},"labels":[],"label_agreement":null},{"id":"W1988149632","doi":"10.1088/0004-637x/718/2/768","title":"INTEGRATED STELLAR POPULATIONS: CONFRONTING PHOTOMETRY WITH SPECTROSCOPY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Photometry (optics); Stellar population; Galaxy; Stars; Asymptotic giant branch; Population; Star formation; Flux (metallurgy); Spiral galaxy; Spectroscopy; Red supergiant; Astronomy; Supergiant; Chemistry","score_opus":0.011963995902739192,"score_gpt":0.24245704541296623,"score_spread":0.23049304951022703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988149632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9113146,0.0008681931,0.08245931,0.00018654962,0.000023674233,0.00006540949,0.00056092406,0.00040717013,0.0041141496],"genre_scores_gemma":[0.97878885,0.00020937374,0.020444442,0.000038221282,0.0000144408505,0.00002444175,0.00027096062,0.00003353777,0.0001757366],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99919873,0.00032179922,0.000031822685,0.00020224405,0.00019605024,0.000049394475],"domain_scores_gemma":[0.9950452,0.0027968592,0.00079719565,0.00072251016,0.0004448536,0.0001934431],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029736653,0.00063121907,0.00043296628,0.0011518016,0.00025813657,0.0012188021,0.0009009127,0.0008895234,0.0005916187],"category_scores_gemma":[0.0125857545,0.00043520992,0.00038954595,0.0011266174,0.000510699,0.0018907647,0.0009891419,0.00048136536,0.00030445537],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035227335,0.00020883122,0.6535569,0.00017230918,0.00033916652,0.00029355273,0.0004493614,0.23640221,0.018853713,0.009657257,0.0003938033,0.07932061],"study_design_scores_gemma":[0.000032560438,0.00034700838,0.20981462,0.00007849479,0.00011477703,0.00037838458,0.00029568598,0.759251,0.0079804165,0.020212378,0.0014253485,0.00006929652],"about_ca_topic_score_codex":0.0030412092,"about_ca_topic_score_gemma":0.0030456795,"teacher_disagreement_score":0.0030412092,"about_ca_system_score_codex":0.0007094358,"about_ca_system_score_gemma":0.00028797484,"threshold_uncertainty_score":0.015726388},"labels":[],"label_agreement":null},{"id":"W1988293147","doi":"10.1086/503025","title":"Density Profiles of Collisionless Equilibria. I. Spherical Isotropic Systems","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Halo; Physics; Isotropy; Power law; Dark matter; Statistical physics; Classical mechanics; Connection (principal bundle); Relaxation (psychology); Phase space; Astrophysics; Quantum mechanics; Mathematics; Geometry; Statistics; Galaxy","score_opus":0.0069401626615593435,"score_gpt":0.20502385987204372,"score_spread":0.19808369721048438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988293147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98327214,0.00016284565,0.0085406555,0.000120642704,0.0000043296695,0.000030659572,0.00019272287,0.00007267062,0.0076033524],"genre_scores_gemma":[0.9983197,0.000047714922,0.00093119126,0.000015449397,0.0000024303656,0.000008293382,0.00014168305,0.000012951825,0.00052071485],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982834,0.000039438608,0.000009536301,0.000027670174,0.000042393483,0.00005257085],"domain_scores_gemma":[0.9991093,0.00015942196,0.00024194576,0.00008815989,0.00023539366,0.00016577166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040284818,0.00022265209,0.00021325283,0.00082068174,0.0005278093,0.0010682971,0.00068637973,0.00033350507,0.0019701836],"category_scores_gemma":[0.0035013934,0.00021862444,0.00019501142,0.00046446334,0.00085048995,0.00066365936,0.0008348035,0.00039995476,0.00035524266],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007150991,0.00029181465,0.14134414,0.00016785065,0.00016781176,0.0010767514,0.002606386,0.48584238,0.047596797,0.2963977,0.003381594,0.020411652],"study_design_scores_gemma":[0.00007342455,0.00018438256,0.054957416,0.000030079393,0.000025520749,0.00047833455,0.00091841316,0.8980025,0.012852958,0.029555237,0.0028520648,0.000069693604],"about_ca_topic_score_codex":0.008752932,"about_ca_topic_score_gemma":0.0038375456,"teacher_disagreement_score":0.008752932,"about_ca_system_score_codex":0.001238188,"about_ca_system_score_gemma":0.00038909385,"threshold_uncertainty_score":0.01740396},"labels":[],"label_agreement":null},{"id":"W1988317071","doi":"10.1086/499328","title":"An Implicit Method for Radiative Transfer with the Diffusion Approximation in Smooth Particle Hydrodynamics","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Fluid Dynamics Simulations and Interactions","field":"Engineering","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Smoothed-particle hydrodynamics; Radiative transfer; Isothermal process; Physics; Heavy traffic approximation; Ideal gas; Radiant energy; Diffusion; Mechanics; Dissociation (chemistry); Equation of state; Statistical physics; Classical mechanics; Thermodynamics; Radiation; Chemistry; Mathematics; Quantum mechanics; Physical chemistry","score_opus":0.004799668296792599,"score_gpt":0.2342644234564456,"score_spread":0.229464755159653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988317071","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0030932266,0.0001585918,0.9938053,0.00008287784,0.000101455684,0.00009563011,0.000097594755,0.0006608645,0.0019043862],"genre_scores_gemma":[0.07069464,0.0003188517,0.9180352,0.00008671926,0.00008870923,0.00051414093,0.00019783637,0.000804162,0.009259684],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996258,0.000116263436,0.000017158838,0.000030793053,0.00017950394,0.000030442],"domain_scores_gemma":[0.99947375,0.00019564918,0.000035884957,0.00009772532,0.00015904389,0.00003794131],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007259325,0.00069141435,0.00078984187,0.00059681066,0.00074175507,0.00065790163,0.0021648812,0.0009231344,0.003718704],"category_scores_gemma":[0.001772282,0.00038484437,0.00079796615,0.00059724256,0.0005094315,0.0008176975,0.0011269158,0.0014717116,0.0017240561],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020504581,0.0002663807,0.0008646742,0.00045722333,0.00013666104,0.00042309627,0.0002742626,0.39910707,0.044487093,0.27988434,0.00894116,0.264953],"study_design_scores_gemma":[0.000042064396,0.000027396267,0.000110043984,0.000011565458,0.000011169268,0.00007108383,0.000006417067,0.971298,0.0028721849,0.0114014195,0.014122707,0.000025955513],"about_ca_topic_score_codex":0.0034608932,"about_ca_topic_score_gemma":0.0020183665,"teacher_disagreement_score":0.003718704,"about_ca_system_score_codex":0.00062943634,"about_ca_system_score_gemma":0.0012701064,"threshold_uncertainty_score":0.012440324},"labels":[],"label_agreement":null},{"id":"W1988410625","doi":"10.1088/0004-637x/691/2/1307","title":"THE X-RAY CLUSTER NORMALIZATION OF THE MATTER POWER SPECTRUM","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Normalization (sociology); Physics; Spectral density; Cluster (spacecraft); Galaxy cluster; Matter power spectrum; Astrophysics; Galaxy; Statistical physics; Statistics; Mathematics","score_opus":0.0031813825154710144,"score_gpt":0.19021636217917806,"score_spread":0.18703497966370705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988410625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6494061,0.00075904606,0.2582678,0.00024325149,0.000111327914,0.00006408731,0.0029547492,0.0015433748,0.08665032],"genre_scores_gemma":[0.96452403,0.0003356219,0.027614143,0.00009329141,0.000054705913,0.000088390996,0.0020582406,0.00023240359,0.00499926],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992836,0.00011475255,0.000029509478,0.00022130147,0.0002909641,0.000059754162],"domain_scores_gemma":[0.9986463,0.00032039496,0.00025246947,0.00043891973,0.00028079396,0.0000610742],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000989009,0.0004275002,0.00033631016,0.0011304375,0.00033402437,0.0011273383,0.00076671055,0.00023645505,0.004251417],"category_scores_gemma":[0.0046694977,0.00020001613,0.00033093517,0.000997415,0.0010875184,0.00096701126,0.0010768741,0.0004302902,0.0018540871],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040122977,0.000054660686,0.4358288,0.0002993161,0.0003968277,0.00029288686,0.0008199385,0.078998685,0.06945494,0.23183593,0.007404592,0.17421208],"study_design_scores_gemma":[0.000017137801,0.00009041247,0.7849429,0.00008721066,0.000048858976,0.0005938514,0.00020948902,0.08678877,0.040182803,0.06445188,0.022499839,0.00008680474],"about_ca_topic_score_codex":0.0036371532,"about_ca_topic_score_gemma":0.003934112,"teacher_disagreement_score":0.004251417,"about_ca_system_score_codex":0.00059847935,"about_ca_system_score_gemma":0.0004391845,"threshold_uncertainty_score":0.014222443},"labels":[],"label_agreement":null},{"id":"W1988421315","doi":"10.1086/504712","title":"A Gamma-Ray Burst Remnant in Our Galaxy: HESS J1303-631","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Supernova remnant; Gamma-ray burst; Supernova; Galaxy; Interstellar medium; Synchrotron radiation; Galactic plane; Observable","score_opus":0.009053922087910858,"score_gpt":0.22965776282729322,"score_spread":0.22060384073938236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988421315","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99934465,0.000036533016,0.00006634443,0.00000936037,7.6494837e-7,0.0000024905023,0.00016836081,0.0000134259735,0.00035806044],"genre_scores_gemma":[0.99835545,0.000053991393,0.00030432193,0.000009135941,0.0000031761417,0.000001562105,0.001129562,0.0000073698498,0.00013539253],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999478,0.000005667655,0.0000033590893,0.000015746355,0.000014767946,0.000012628984],"domain_scores_gemma":[0.99974805,0.000033847668,0.000096674405,0.000037742448,0.000019360123,0.0000644488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013623832,0.00022917522,0.0002329299,0.0005879598,0.00026944603,0.0005091623,0.00021276863,0.00019788208,0.00049568096],"category_scores_gemma":[0.00032329993,0.00011156411,0.00018108507,0.0007270315,0.00024216516,0.00019532128,0.00041694893,0.00020060937,0.00026265395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061957777,0.00015250423,0.9425346,0.00006123557,0.00014185869,0.004394043,0.00086902705,0.0036419437,0.034663584,0.00048305048,0.00069544214,0.0117431935],"study_design_scores_gemma":[0.000026582671,0.00012976362,0.9900682,0.0000059802137,0.00005839045,0.0010703886,0.00024928694,0.0038261309,0.003077024,0.00015186596,0.0013188411,0.000017578586],"about_ca_topic_score_codex":0.013048493,"about_ca_topic_score_gemma":0.012866738,"teacher_disagreement_score":0.013048493,"about_ca_system_score_codex":0.0003433085,"about_ca_system_score_gemma":0.0001853199,"threshold_uncertainty_score":0.025945127},"labels":[],"label_agreement":null},{"id":"W1988495425","doi":"10.1086/424794","title":"Distance of Three Supernova Remnants from H<scp>i</scp>Line Observations in a Complex Region: G114.3+0.3, G116.5+1.1, and CTB 1 (G116.9+0.2)","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Supernova; Breakout; Galactic plane; Astronomy; Line (geometry); Bubble; Star (game theory); Stars; Geometry","score_opus":0.03810015474354777,"score_gpt":0.23622442630553817,"score_spread":0.1981242715619904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988495425","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99927837,0.0000520913,0.00005449285,0.000013959944,0.0000038738976,0.0000036512217,0.00014877222,0.000027232825,0.0004175461],"genre_scores_gemma":[0.9989962,0.000024751658,0.00012978914,0.000008716768,0.000003347055,0.0000020054226,0.0006774113,0.0000062851136,0.00015145133],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986756,0.000007439093,0.000007317917,0.000040132414,0.000034617853,0.00004300347],"domain_scores_gemma":[0.99950576,0.000024785122,0.00013068173,0.00003371815,0.000039294093,0.00026575307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018409238,0.00031489666,0.00025046626,0.0008583614,0.00058976474,0.0006688643,0.0003686719,0.00051841885,0.00094408996],"category_scores_gemma":[0.0004014659,0.00022226138,0.00026652412,0.0004670457,0.000417173,0.00017824327,0.000848227,0.00033451832,0.0002942078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007515121,0.000098919445,0.9351236,0.0000464389,0.00014990561,0.0020901544,0.00080364395,0.00060330605,0.04929428,0.0001398079,0.0007458345,0.010152474],"study_design_scores_gemma":[0.000004640132,0.00002290335,0.99865025,0.0000026873008,0.000011956236,0.00018817453,0.000072587056,0.00016622395,0.00062596035,0.000008446122,0.0002426302,0.0000035963349],"about_ca_topic_score_codex":0.036254954,"about_ca_topic_score_gemma":0.050893284,"teacher_disagreement_score":0.036254954,"about_ca_system_score_codex":0.00074567756,"about_ca_system_score_gemma":0.00025621496,"threshold_uncertainty_score":0.072087824},"labels":[],"label_agreement":null},{"id":"W1988574878","doi":"10.1088/0004-637x/763/1/4","title":"PAndAS IN THE MIST: THE STELLAR AND GASEOUS MASS WITHIN THE HALOS OF M31 AND M33","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto; Queen's University; Dominion Astrophysical Observatory","funders":"Science and Technology Facilities Council","keywords":"Substructure; Halo; Stars; Spiral galaxy; Accretion (finance); Milky Way; Galaxy; Local Group","score_opus":0.007774577128993777,"score_gpt":0.20544499688200885,"score_spread":0.19767041975301508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988574878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99935895,0.00005897724,0.000018438845,0.000032835418,7.232178e-7,6.433402e-7,0.000030241821,0.0000016890922,0.0004974822],"genre_scores_gemma":[0.9998215,0.000021132442,0.000028817158,0.0000078912335,0.0000011542746,3.676674e-7,0.000046468474,0.0000013169163,0.000071307644],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999325,0.000013957842,0.0000027305139,0.000016250287,0.000013173773,0.000021244701],"domain_scores_gemma":[0.9997329,0.000022919174,0.000085911626,0.000034280776,0.000032939526,0.000091044145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001622632,0.00008244439,0.00011990118,0.0005414023,0.0005366768,0.000541583,0.00013498338,0.00012554457,0.0009829121],"category_scores_gemma":[0.00066418137,0.00007158505,0.00008586413,0.00057439815,0.00041823855,0.00039280285,0.0007641864,0.00014432908,0.00022514483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015801592,0.000013448078,0.9820514,0.000008646844,0.000022624234,0.00015391728,0.0015073096,0.00010284812,0.006643351,0.0009324678,0.00022358577,0.008182402],"study_design_scores_gemma":[0.0000016048613,0.000012280075,0.99834085,0.0000022378674,0.0000046990344,0.00010619581,0.00062050845,0.00015298424,0.0001575014,0.00015700981,0.00044238108,0.0000017680819],"about_ca_topic_score_codex":0.013899784,"about_ca_topic_score_gemma":0.023331203,"teacher_disagreement_score":0.013899784,"about_ca_system_score_codex":0.0003150654,"about_ca_system_score_gemma":0.00021951635,"threshold_uncertainty_score":0.02763772},"labels":[],"label_agreement":null},{"id":"W1988594587","doi":"10.1086/379360","title":"The DEEP Groth Strip Survey. VII. The Metallicity of Field Galaxies at 0.26 &lt;<i>z</i>&lt; 0.82 and the Evolution of the Luminosity‐Metallicity Relation","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Metallicity; Galaxy; Relation (database); Field (mathematics); Disc galaxy; Galaxy formation and evolution; Galaxy group","score_opus":0.007010955409918744,"score_gpt":0.195730022210378,"score_spread":0.18871906680045925,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988594587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.62750524,0.0024096922,0.00047715637,0.0018673579,0.00029599844,0.00007089919,0.35148653,0.00023941808,0.015647663],"genre_scores_gemma":[0.78140944,0.00089129043,0.0011711926,0.000690584,0.00023142017,0.00009541604,0.19459993,0.0000739238,0.020836702],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999877,0.000015189894,0.000011519618,0.000025261683,0.000026565192,0.00004444651],"domain_scores_gemma":[0.99894863,0.00010727868,0.00025432452,0.000116225354,0.0002259198,0.00034761362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000425334,0.00028662663,0.00021357209,0.001480831,0.00022584209,0.0005685466,0.00047283954,0.00046112167,0.005142433],"category_scores_gemma":[0.0009901059,0.00029800477,0.00028956283,0.0015748738,0.0002217944,0.00034899265,0.0007158792,0.00037886755,0.0026635742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049908116,0.0000701307,0.8890109,0.00021258436,0.00026167385,0.00022917603,0.00029085588,0.0003334552,0.0025450431,0.00041655335,0.08491058,0.021220008],"study_design_scores_gemma":[0.00002078793,0.000016014626,0.9932569,0.000010624019,0.000028497558,0.000035033045,0.000060928276,0.000028072309,0.00012187545,0.00005293743,0.006364966,0.0000031533286],"about_ca_topic_score_codex":0.06617483,"about_ca_topic_score_gemma":0.12097143,"teacher_disagreement_score":0.06617483,"about_ca_system_score_codex":0.00035636948,"about_ca_system_score_gemma":0.00037146814,"threshold_uncertainty_score":0.13157928},"labels":[],"label_agreement":null},{"id":"W1988634165","doi":"10.1086/426965","title":"Flickering Red Giants in the Ursa Minor Dwarf Spheroidal Galaxy: Detection of Low-Amplitude Variability in Faint Red Giant Branch Stars on 10 Minute Timescales","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Red-giant branch; Astrophysics; Astronomy; Red giant; Stars; Brightness; Asymptotic giant branch; Giant star; Amplitude; Red clump; Galaxy; Photometry (optics); Horizontal branch; Globular cluster; Milky Way","score_opus":0.010760579772194107,"score_gpt":0.22126012583448007,"score_spread":0.21049954606228596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988634165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997497,0.000028686223,0.00009741142,0.0000046087525,7.6634956e-7,0.000001449539,0.000040255625,0.000006820069,0.000070334325],"genre_scores_gemma":[0.9994942,0.00002028234,0.0001989214,0.0000069437874,0.0000032075257,0.0000024631943,0.00017875571,0.0000022259642,0.0000929188],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998791,0.000018200068,0.000010565878,0.000032446645,0.00002845364,0.000031093427],"domain_scores_gemma":[0.9991943,0.00011555492,0.00030959747,0.00007645825,0.00012408706,0.00018001864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024736446,0.0001489674,0.000252428,0.00070507755,0.00024296908,0.00028786584,0.00021045904,0.00020857819,0.00040907424],"category_scores_gemma":[0.0009868447,0.00014121126,0.00012166329,0.0003829127,0.0002312521,0.00020018862,0.0003527778,0.0001601121,0.00011938812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016986797,0.000044886052,0.9112363,0.000023266797,0.000036128647,0.0003236961,0.00045980982,0.00018379076,0.08058844,0.000051465595,0.00008552641,0.0067969006],"study_design_scores_gemma":[0.0000019802326,0.000043044103,0.998192,0.0000011808349,0.000008213513,0.00017767424,0.000037811787,0.00016481448,0.0012659912,0.0000108197955,0.000093858136,0.0000024678661],"about_ca_topic_score_codex":0.0021923492,"about_ca_topic_score_gemma":0.006836632,"teacher_disagreement_score":0.0021923492,"about_ca_system_score_codex":0.00021557296,"about_ca_system_score_gemma":0.00008695824,"threshold_uncertainty_score":0.0043592453},"labels":[],"label_agreement":null},{"id":"W1988752970","doi":"10.1086/500653","title":"Multiwavelength Observations of the Blazar Markarian 421 in 2002 December and 2003 January","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Blazar; Astrophysics; Flare; Crab Nebula; Light curve; Flux (metallurgy); Telescope; Sky; Spectral index; Astronomy; Observatory; Active galactic nucleus; Synchrotron; Gamma ray; Spectral line; Galaxy","score_opus":0.008551485056337389,"score_gpt":0.1999201054443607,"score_spread":0.19136862038802332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988752970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954094,0.0002742922,0.00018675141,0.00007853562,0.000010380288,0.000020008758,0.00068767887,0.00005946309,0.0032735441],"genre_scores_gemma":[0.99128,0.00029223744,0.0010246448,0.00011231708,0.000052660987,0.000027795337,0.0047091832,0.000044055952,0.0024569803],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970716,0.000025076857,0.000015156538,0.00007094401,0.000098720004,0.000082928345],"domain_scores_gemma":[0.9995783,0.000017141616,0.00017505873,0.000041656534,0.00007349258,0.00011435033],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032358328,0.00031841788,0.0005407654,0.0009781767,0.00076780474,0.00087446644,0.00036991798,0.00050376274,0.0005964692],"category_scores_gemma":[0.00048082997,0.0002588217,0.00025479135,0.0008525151,0.00014879422,0.00027366375,0.00071404706,0.00042510277,0.0005469746],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014965319,0.00047027614,0.820258,0.00020237012,0.00036214417,0.0037446425,0.0048853667,0.0010328453,0.12189277,0.00043579127,0.005880255,0.03933901],"study_design_scores_gemma":[0.000012661095,0.00007627357,0.9930046,0.00000722268,0.000021762753,0.0004155499,0.00017975774,0.0001465761,0.0011841094,0.000019698375,0.0049229064,0.00000877677],"about_ca_topic_score_codex":0.010878387,"about_ca_topic_score_gemma":0.03759139,"teacher_disagreement_score":0.010878387,"about_ca_system_score_codex":0.00048305065,"about_ca_system_score_gemma":0.00029954407,"threshold_uncertainty_score":0.021630108},"labels":[],"label_agreement":null},{"id":"W1988887435","doi":"10.1086/319495","title":"Possible Local Spiral Galaxy Counterparts to Compact Blue Galaxies at Intermediate Redshift","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Spiral galaxy; Redshift; Galaxy; Elliptical galaxy; Compact group; Irregular galaxy; Star formation; Blueshift; Lenticular galaxy","score_opus":0.009086811608644154,"score_gpt":0.22967152145226014,"score_spread":0.22058470984361597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988887435","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976532,0.00020933282,0.00043167325,0.00003050523,0.0000022560873,0.0000043532823,0.000052928383,0.000023277289,0.0015924353],"genre_scores_gemma":[0.9994306,0.000037121004,0.00017174911,0.000007708102,0.00000458418,0.0000021910469,0.00006935394,0.0000017004854,0.0002749906],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999238,0.0000066583452,0.0000043867803,0.000023892024,0.000010581254,0.000030613435],"domain_scores_gemma":[0.99905294,0.00010916941,0.000380404,0.00011128946,0.00007854161,0.0002676683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021715916,0.00028014288,0.0002484619,0.0010522347,0.0004312969,0.00067933224,0.00028938593,0.00024493755,0.0034043996],"category_scores_gemma":[0.0010491477,0.00016090658,0.000114143724,0.0006446387,0.00057468895,0.00040694803,0.00053540966,0.000173108,0.0006098624],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000473271,0.000065765315,0.9528622,0.00005495794,0.000035411613,0.0018491304,0.0019303132,0.00022126095,0.017351246,0.0042152405,0.00028423287,0.020657096],"study_design_scores_gemma":[0.00006919082,0.00039702308,0.97330296,0.00003811974,0.00008899236,0.009266437,0.0021875883,0.001117494,0.003144871,0.006183288,0.0041846843,0.000019367504],"about_ca_topic_score_codex":0.0010246348,"about_ca_topic_score_gemma":0.0023609542,"teacher_disagreement_score":0.0034043996,"about_ca_system_score_codex":0.00023124901,"about_ca_system_score_gemma":0.00007572279,"threshold_uncertainty_score":0.011388898},"labels":[],"label_agreement":null},{"id":"W1988969529","doi":"10.1088/0004-637x/749/1/69","title":"CONSTRAINTS ON NEUTRON STAR MASS AND RADIUS IN GS 1826–24 FROM SUB-EDDINGTON X-RAY BURSTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Neutron star; Photosphere; Luminosity; Black-body radiation; RADIUS; Metallicity; Stellar mass; Light curve; Spectral line; Astronomy; Radiation; Star formation; Stars; Galaxy; Optics","score_opus":0.013519600803272183,"score_gpt":0.22723230491159893,"score_spread":0.21371270410832674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988969529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99862564,0.000088154105,0.00019843642,0.000024277639,0.0000018248612,0.0000012425949,0.00016620957,0.000016873706,0.0008774116],"genre_scores_gemma":[0.9985654,0.00009030719,0.00032006082,0.000007966234,0.000007214691,0.0000022445934,0.00070318434,0.000016233642,0.00028740347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991405,0.0000130662265,0.0000066471525,0.000029026894,0.000020785163,0.000016464228],"domain_scores_gemma":[0.99965763,0.00006113394,0.00013322735,0.000053179174,0.00002365925,0.000071146256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001988082,0.0005211875,0.00044052713,0.0007245975,0.00031305602,0.00059721863,0.00040735697,0.00028000562,0.0010456184],"category_scores_gemma":[0.0007339599,0.00025493762,0.00035601328,0.00056710537,0.00028202115,0.00030792033,0.00069650006,0.00023343146,0.00040701538],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005593585,0.00006110773,0.8916172,0.00009785457,0.00010337869,0.0011311077,0.000559882,0.04565397,0.04589733,0.0021858562,0.0006681878,0.011464722],"study_design_scores_gemma":[0.00003192141,0.0001330664,0.9443583,0.000026237583,0.000038322898,0.00061839825,0.00027157742,0.044866357,0.0045010718,0.0018467158,0.0032694929,0.000038730588],"about_ca_topic_score_codex":0.004306759,"about_ca_topic_score_gemma":0.005673982,"teacher_disagreement_score":0.004306759,"about_ca_system_score_codex":0.0006676039,"about_ca_system_score_gemma":0.00018018823,"threshold_uncertainty_score":0.008563399},"labels":[],"label_agreement":null},{"id":"W1988991313","doi":"10.1088/0004-637x/706/1/184","title":"MILLIMETER OBSERVATIONS OF A SAMPLE OF HIGH-REDSHIFT OBSCURED QUASARS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Redshift; Quasar; Luminosity; Plateau de Bure Interferometer; Active galactic nucleus; Extinction (optical mineralogy); Star formation; Infrared; Astronomy; Spectral energy distribution; Cosmic infrared background; Galaxy; Cosmic microwave background","score_opus":0.016161810350200943,"score_gpt":0.224977045051609,"score_spread":0.20881523470140806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1988991313","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978994,0.00017545439,0.00071461895,0.000023006864,0.000004667312,0.000009411852,0.0005847035,0.000060857237,0.0005279692],"genre_scores_gemma":[0.99612087,0.00014860269,0.0015678398,0.000030023306,0.000031090614,0.000013424232,0.0018110974,0.000008040743,0.0002690098],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998078,0.000019411305,0.000013778363,0.00004726505,0.00004736098,0.00006437635],"domain_scores_gemma":[0.99937505,0.00009024949,0.00027667775,0.000095136646,0.000049594706,0.000113357884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003119177,0.0003553739,0.0003193905,0.0010191299,0.00028732375,0.0004787792,0.0003584534,0.0002851553,0.00062774785],"category_scores_gemma":[0.00047678896,0.00023223048,0.00024177322,0.0011330583,0.00016474689,0.00020550695,0.0005934239,0.00029554486,0.0002048078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033167674,0.00013897149,0.91126186,0.0000635458,0.00020245857,0.0005663451,0.00047372552,0.00088763796,0.06740195,0.00040310682,0.0008513409,0.017417317],"study_design_scores_gemma":[0.000009771098,0.000050767194,0.997352,0.0000018651242,0.000023404265,0.00021882153,0.000048970054,0.000298046,0.0011829933,0.000035115976,0.00077430916,0.000003851165],"about_ca_topic_score_codex":0.0018718374,"about_ca_topic_score_gemma":0.0034316925,"teacher_disagreement_score":0.0018718374,"about_ca_system_score_codex":0.00017885768,"about_ca_system_score_gemma":0.000088679786,"threshold_uncertainty_score":0.0037218332},"labels":[],"label_agreement":null},{"id":"W1989041145","doi":"10.1088/0004-637x/787/2/166","title":"INVESTIGATING THE TeV MORPHOLOGY OF MGRO J1908+06 WITH VERITAS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Energy spectrum; High energy; X-ray pulsar; Binary pulsar; Gamma-ray astronomy; Measure (data warehouse)","score_opus":0.007857278608827956,"score_gpt":0.20667449091016893,"score_spread":0.19881721230134097,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989041145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971534,0.00008947242,0.0003222846,0.00002629609,0.000004654377,0.0000047056537,0.00033103867,0.000033534627,0.0020345321],"genre_scores_gemma":[0.995545,0.00009250411,0.0018343189,0.000062121144,0.000020725729,0.0000051130924,0.0015511318,0.000038878126,0.00085009035],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988437,0.0000063192756,0.0000038248304,0.000035962992,0.00004049803,0.000028997505],"domain_scores_gemma":[0.9995809,0.000041058323,0.0001853796,0.00006017625,0.000051711086,0.00008068184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017699288,0.00016588814,0.00024305227,0.0006090716,0.0002850819,0.00049832044,0.00040635304,0.00023172949,0.00116652],"category_scores_gemma":[0.00038669622,0.0001795581,0.0001656504,0.00050337135,0.00022294141,0.00023340207,0.0006193662,0.00029017442,0.00037056478],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005120093,0.000121285615,0.6479959,0.00005827028,0.0001018257,0.0025382366,0.0005626423,0.0007307291,0.32165647,0.00055562,0.0009506376,0.024216399],"study_design_scores_gemma":[0.000013987265,0.00012846071,0.9909746,0.000006821674,0.000020305019,0.001432658,0.00011837742,0.0008591014,0.0033214353,0.00007528417,0.0030420094,0.000006974327],"about_ca_topic_score_codex":0.0032353804,"about_ca_topic_score_gemma":0.011370352,"teacher_disagreement_score":0.0032353804,"about_ca_system_score_codex":0.00027586686,"about_ca_system_score_gemma":0.00012594613,"threshold_uncertainty_score":0.0064330697},"labels":[],"label_agreement":null},{"id":"W1989229046","doi":"10.1086/338698","title":"Long‐Term<i>Rossi X‐Ray Timing Explorer</i>Monitoring of Anomalous X‐Ray Pulsars","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Astrophysics; Glitch; Static timing analysis; Ephemeris; Pulse (music); Flux (metallurgy); Phase (matter); Vela; Stability (learning theory); X-ray pulsar; Coherence (philosophical gambling strategy); Astronomy; Satellite; Optics; Detector","score_opus":0.03333084770763403,"score_gpt":0.31581845126035407,"score_spread":0.28248760355272007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989229046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947221,0.00021941299,0.001638867,0.0000714528,0.000009385779,0.00001373069,0.0011270016,0.00011843997,0.0020795718],"genre_scores_gemma":[0.99082726,0.00019836688,0.0051444406,0.00007421872,0.000042116455,0.00003300699,0.0027953559,0.000053532836,0.0008317975],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998541,0.000014575166,0.0000099673825,0.000037536596,0.000050187908,0.00003354736],"domain_scores_gemma":[0.99939394,0.000052005293,0.0002671414,0.000062618405,0.00011921398,0.00010503224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038783107,0.00023166918,0.00019349414,0.000740938,0.00027798378,0.00034961503,0.00029661952,0.00025119423,0.00042351033],"category_scores_gemma":[0.000548503,0.00009153999,0.00019724519,0.00043672015,0.00017230518,0.00023996674,0.000532499,0.00030849566,0.00019740041],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003022365,0.00008835518,0.6974476,0.00011210942,0.00019510712,0.00063483365,0.00035410016,0.0018440987,0.24445423,0.00040025453,0.001633678,0.05253343],"study_design_scores_gemma":[0.000007783084,0.0001905258,0.9799081,0.000009344155,0.00004428195,0.0005691474,0.000055919852,0.0019984364,0.014245955,0.0001016157,0.0028471525,0.000021740052],"about_ca_topic_score_codex":0.0017894572,"about_ca_topic_score_gemma":0.005559402,"teacher_disagreement_score":0.0017894572,"about_ca_system_score_codex":0.00017217397,"about_ca_system_score_gemma":0.00013386425,"threshold_uncertainty_score":0.0035580993},"labels":[],"label_agreement":null},{"id":"W1989357618","doi":"10.1088/0004-637x/745/1/101","title":"SPIN EVOLUTION OF ACCRETING YOUNG STARS. II. EFFECT OF ACCRETION-POWERED STELLAR WINDS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Accretion (finance); Stellar rotation; Stars; Angular momentum; Outflow; Intermediate polar; T Tauri star; Astronomy; Stellar mass; Spin (aerodynamics); Stellar evolution; Star formation; White dwarf; Classical mechanics","score_opus":0.006679929350234293,"score_gpt":0.2440906695813124,"score_spread":0.2374107402310781,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989357618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965519,0.0004963197,0.00034826586,0.000055073662,0.000014769452,0.000006334271,0.00017314112,0.00001899871,0.0023351759],"genre_scores_gemma":[0.9984592,0.0002246053,0.000105132036,0.000017767275,0.000012313547,0.0000025230854,0.0001727344,0.0000146203565,0.0009910694],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999515,0.000010998304,0.0000031134086,0.000008673881,0.000006747563,0.000018992188],"domain_scores_gemma":[0.9994917,0.00018605978,0.00010010521,0.00004393229,0.00006350319,0.00011467306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025176318,0.00023834144,0.00034796444,0.00033423942,0.0003490374,0.00063660037,0.0001863789,0.00034244667,0.0018214519],"category_scores_gemma":[0.0010857023,0.00015334057,0.00036245806,0.00021457388,0.00029369662,0.0002691474,0.00040481612,0.00037127853,0.0005482412],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.005576832,0.00057771924,0.6679362,0.00033055205,0.00037020817,0.0032403641,0.0007328965,0.061238922,0.19707866,0.006230794,0.0026116548,0.05407523],"study_design_scores_gemma":[0.00017334837,0.0007516379,0.88989407,0.000040116167,0.00011935554,0.0007359143,0.0005337459,0.0874087,0.016173108,0.002969394,0.0011459503,0.000054801454],"about_ca_topic_score_codex":0.0021421297,"about_ca_topic_score_gemma":0.0025741004,"teacher_disagreement_score":0.0021421297,"about_ca_system_score_codex":0.00030045418,"about_ca_system_score_gemma":0.00011029142,"threshold_uncertainty_score":0.006093383},"labels":[],"label_agreement":null},{"id":"W1989361110","doi":"10.1088/0004-637x/781/2/73","title":"SEARCHING FOR MAGNETIC FIELDS IN 11 WOLF-RAYET STARS: ANALYSIS OF CIRCULAR POLARIZATION MEASUREMENTS FROM ESPaDOnS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Stars; Astrophysics; Wolf–Rayet star; Neutron star; Magnetic field; K-type main-sequence star; Astronomy; T Tauri star","score_opus":0.01982393555191929,"score_gpt":0.24394763596881816,"score_spread":0.22412370041689889,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989361110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988984,0.000030891522,0.0001244824,0.000004954957,8.426813e-7,0.0000039522183,0.00026448703,0.0000036647543,0.0006682205],"genre_scores_gemma":[0.997442,0.000062166066,0.00041606772,0.000013942133,0.000003141391,0.000004826596,0.001747006,0.000003536147,0.00030741483],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999788,0.000022978105,0.000027189375,0.00007682786,0.00005882434,0.0000261546],"domain_scores_gemma":[0.99950814,0.000070606475,0.00010126042,0.000049821097,0.00015239745,0.000117762276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040823416,0.0002959038,0.00025395173,0.0014798626,0.00030769553,0.00045662746,0.00027686203,0.0002539084,0.0005571892],"category_scores_gemma":[0.00063286966,0.00015528518,0.00018972736,0.0007117019,0.00021007369,0.00016518054,0.00057751103,0.00014489706,0.00030997154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010987129,0.000025455674,0.98288524,0.000018529838,0.000047902675,0.00033297171,0.00018232602,0.00026359718,0.010518232,0.000048327118,0.00008598586,0.0054816143],"study_design_scores_gemma":[0.0000048540915,0.000023994175,0.9981104,0.0000034540951,0.000013367347,0.00012998942,0.00021387164,0.00031475013,0.00072011334,0.000023488543,0.0004388231,0.000002960432],"about_ca_topic_score_codex":0.005870345,"about_ca_topic_score_gemma":0.0105135925,"teacher_disagreement_score":0.005870345,"about_ca_system_score_codex":0.00029259184,"about_ca_system_score_gemma":0.00014958631,"threshold_uncertainty_score":0.011672318},"labels":[],"label_agreement":null},{"id":"W1989368763","doi":"10.1086/309129","title":"Interstellar Clump Behavior and Magnetic Effects in Small Clumps","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Interstellar medium; Magnetic field; Line (geometry); Molecular cloud; Resolution (logic); Astronomy; Stars; Galaxy","score_opus":0.006231793390456735,"score_gpt":0.2138365929105873,"score_spread":0.20760479952013056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989368763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993998,0.00016686431,0.000079591206,0.000008110564,0.0000019804177,0.0000020929074,0.000019345442,0.0000044805915,0.00031776426],"genre_scores_gemma":[0.9997924,0.00002981822,0.00004258471,0.0000042875363,0.0000024361711,0.0000012909566,0.000030780484,0.0000019160937,0.000094534465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999269,0.0000071866234,0.0000057707166,0.00002347926,0.000017586244,0.000019093712],"domain_scores_gemma":[0.9990081,0.0002239312,0.00033272043,0.00007872789,0.00013953913,0.00021695362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016300648,0.00009946845,0.00017945233,0.0005910633,0.000246123,0.0005174845,0.00025929493,0.00020057934,0.00074724],"category_scores_gemma":[0.0014061916,0.000113099806,0.00008405902,0.0002482734,0.00032745284,0.00026533552,0.00036588064,0.00015859856,0.00018249395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001183621,0.00018216587,0.63682365,0.00011348623,0.00009910555,0.0012864257,0.00097139145,0.0032192017,0.3357036,0.0011436732,0.00050261314,0.018771015],"study_design_scores_gemma":[0.00005878897,0.0003549515,0.9712225,0.000013757926,0.000036460668,0.00054538937,0.00034824357,0.006415064,0.01981623,0.00050221203,0.0006658351,0.000020480862],"about_ca_topic_score_codex":0.0013399337,"about_ca_topic_score_gemma":0.0010644535,"teacher_disagreement_score":0.0013399337,"about_ca_system_score_codex":0.000248711,"about_ca_system_score_gemma":0.00008958814,"threshold_uncertainty_score":0.0026642084},"labels":[],"label_agreement":null},{"id":"W1989402773","doi":"10.1088/0004-637x/778/1/65","title":"ON THE THERMAL STABILITY OF RADIATION-DOMINATED ACCRETION DISKS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Magnetohydrodynamics; Dynamo; Turbulence; Dissipation; Advection; Thermal; Thermal radiation; Accretion (finance); Adiabatic process","score_opus":0.010480386129856722,"score_gpt":0.22841221953011462,"score_spread":0.2179318334002579,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989402773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903752,0.00059121556,0.00560765,0.00020234076,0.000018753828,0.000011249041,0.00006141829,0.00005952235,0.0030725817],"genre_scores_gemma":[0.9987759,0.00015731734,0.0006332451,0.000025000296,0.000017833234,0.000009269388,0.000040584095,0.000021462585,0.00031949425],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998648,0.00004453847,0.000007295056,0.000029762878,0.000020136073,0.000033479868],"domain_scores_gemma":[0.9991436,0.00041381523,0.00020888458,0.000055781682,0.000099838995,0.00007804107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043197215,0.0005824452,0.0005072158,0.0005656168,0.00067228585,0.00092015584,0.00083063694,0.00070623326,0.00068717956],"category_scores_gemma":[0.0028688468,0.0002628105,0.00046174318,0.00041911178,0.0010934273,0.000996023,0.0009846906,0.00045649317,0.00014143198],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001999204,0.000082182094,0.01725118,0.000086354405,0.00013076971,0.00058198295,0.0002329742,0.9587157,0.0131086875,0.005625851,0.0003749076,0.0036094387],"study_design_scores_gemma":[0.000018108092,0.000041922674,0.003356827,0.000008056825,0.000015923211,0.000029822782,0.000037707334,0.9936172,0.0010591832,0.0016839753,0.00011862972,0.00001264257],"about_ca_topic_score_codex":0.0051863045,"about_ca_topic_score_gemma":0.0015840855,"teacher_disagreement_score":0.0051863045,"about_ca_system_score_codex":0.00066006364,"about_ca_system_score_gemma":0.00032500332,"threshold_uncertainty_score":0.010312259},"labels":[],"label_agreement":null},{"id":"W1989442936","doi":"10.1086/338888","title":"Photon‐dominated Regions in Low‐Ultraviolet Fields: A Study of the Peripheral Region of L1204/S140","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"CMC Microsystems (Canada)","funders":"","keywords":"Photoionization; Physics; Ultraviolet; Astrophysics; Molecular cloud; Infrared; Photon; Radiation; Atomic physics; Astronomy; Ion; Optics; Ionization; Quantum mechanics","score_opus":0.01463476016754006,"score_gpt":0.23304334919294478,"score_spread":0.21840858902540472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989442936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985959,0.000080580125,0.00016040746,0.000018128929,0.0000010501134,0.0000050667336,0.00010316129,0.00002326997,0.0010124735],"genre_scores_gemma":[0.9988714,0.00005862241,0.0003487277,0.000022899532,0.000006432401,0.000005606567,0.0004144512,0.0000143513735,0.00025757428],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999,0.0000074927716,0.000002332051,0.000026509417,0.000025063593,0.000038558028],"domain_scores_gemma":[0.99976057,0.000038235125,0.000064574815,0.000013316263,0.000036957175,0.00008636574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015653677,0.00033573192,0.00044532094,0.00078694685,0.00076518214,0.0005682912,0.0006144148,0.00029867262,0.0015233278],"category_scores_gemma":[0.00027928976,0.0003099981,0.00026303562,0.00073699583,0.00040462922,0.00045933764,0.0006910728,0.00038850735,0.00026539396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011680437,0.00071337813,0.5005054,0.000216857,0.00017911609,0.0019692157,0.0015247404,0.004797085,0.46454376,0.00079189026,0.0007127957,0.022877792],"study_design_scores_gemma":[0.000041886982,0.0002817578,0.98842186,0.000010917946,0.000025207695,0.00030354902,0.00037038288,0.003946298,0.0055026966,0.00014440739,0.00093571265,0.000015413241],"about_ca_topic_score_codex":0.0099750245,"about_ca_topic_score_gemma":0.009563044,"teacher_disagreement_score":0.0099750245,"about_ca_system_score_codex":0.0006086276,"about_ca_system_score_gemma":0.00027584843,"threshold_uncertainty_score":0.019833922},"labels":[],"label_agreement":null},{"id":"W1989468664","doi":"10.1086/517902","title":"Colliding Winds in Symbiotic Binary Systems. II. Colliding Winds Geometries and Orbital Motion in the Symbiotic Nova AG Pegasi","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Royal Military College of Canada","funders":"","keywords":"Physics; Astrophysics; Nebula; Orbital motion; Roche lobe; Stars; Astronomy; Angular momentum; Binary star","score_opus":0.01894384855097814,"score_gpt":0.27371037093079775,"score_spread":0.2547665223798196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989468664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99931467,0.00016783028,0.00009922566,0.000011058665,0.0000010890025,0.0000015502412,0.000020935766,0.0000020299506,0.0003815798],"genre_scores_gemma":[0.9996357,0.0000746162,0.00013412713,0.0000032483308,0.0000015563442,0.0000015440014,0.000063198524,9.2014795e-7,0.00008504079],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999217,0.0000116960255,0.0000057453276,0.000022272443,0.000017692772,0.000021010927],"domain_scores_gemma":[0.9996724,0.000048658283,0.00018857906,0.000020870584,0.000018006587,0.000051570336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013616054,0.00015199228,0.0001794886,0.00044090438,0.0004961648,0.000576072,0.00019469947,0.00030136044,0.0004989885],"category_scores_gemma":[0.00091283204,0.00017537111,0.0001301823,0.00036385845,0.00032345808,0.00047637528,0.00063300354,0.0002538631,0.00011402775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015988457,0.000023801898,0.9741391,0.000024539495,0.000028245564,0.0005778133,0.0005298522,0.002095751,0.011917611,0.00080440694,0.00009146669,0.00960751],"study_design_scores_gemma":[0.0000092721175,0.000057497135,0.99175006,0.0000071037575,0.000011567334,0.0007188818,0.00026884305,0.005333329,0.0004890599,0.00067554624,0.0006733237,0.0000055610662],"about_ca_topic_score_codex":0.0055579282,"about_ca_topic_score_gemma":0.0074658357,"teacher_disagreement_score":0.0055579282,"about_ca_system_score_codex":0.00059857237,"about_ca_system_score_gemma":0.00010715422,"threshold_uncertainty_score":0.011051118},"labels":[],"label_agreement":null},{"id":"W1989476261","doi":"10.1086/506612","title":"The Discovery of Cepheids and a Distance to NGC 5128","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Distance modulus; Astrophysics; Physics; Centaurus A; Galaxy; Population; Astronomy; Metallicity; Luminosity; Spiral galaxy; Radio galaxy; Stars","score_opus":0.004912051782065029,"score_gpt":0.2044611542083291,"score_spread":0.19954910242626409,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989476261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926099,0.00040465445,0.0007036439,0.00013576892,0.000019338906,0.00000371634,0.00011760494,0.000015781532,0.005989686],"genre_scores_gemma":[0.99704176,0.00022533504,0.0011850273,0.000036038582,0.000030693867,0.0000044398803,0.00020680371,0.0000050708554,0.0012648917],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999811,0.0000149500165,0.000012131973,0.00007315797,0.00005213711,0.000036726127],"domain_scores_gemma":[0.999405,0.00008938876,0.00020370695,0.000094883704,0.00007171432,0.00013525094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001723895,0.00019557733,0.00012971887,0.000776516,0.0005630393,0.0008715729,0.00024447558,0.00030366165,0.0015416516],"category_scores_gemma":[0.0010559835,0.00012802883,0.00009105315,0.00060808985,0.00069102965,0.00077052956,0.0009294483,0.00045030034,0.00025698266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002663667,0.000038845912,0.88126314,0.00008438642,0.000028836737,0.0022283646,0.0029669057,0.00045669707,0.028645394,0.010798979,0.0011393557,0.07208271],"study_design_scores_gemma":[0.0000049988453,0.00005360496,0.9824041,0.000028894963,0.000009620542,0.0016955787,0.00041530412,0.0003192571,0.0010300822,0.0018890742,0.012129954,0.000019502093],"about_ca_topic_score_codex":0.0029673695,"about_ca_topic_score_gemma":0.0055955234,"teacher_disagreement_score":0.0029673695,"about_ca_system_score_codex":0.00047495207,"about_ca_system_score_gemma":0.00018320476,"threshold_uncertainty_score":0.0059001446},"labels":[],"label_agreement":null},{"id":"W1989483564","doi":"10.1086/518499","title":"Rotation Measures of Extragalactic Sources behind the Southern Galactic Plane: New Insights into the Large‐Scale Magnetic Field of the Inner Milky Way","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":212,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Pulsar; Milky Way; Galactic plane; Spiral galaxy; Clockwise; Faraday effect; Magnetic field; Galactic Center","score_opus":0.010665824447538984,"score_gpt":0.2760592757365401,"score_spread":0.2653934512890011,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989483564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747556,0.00021702649,0.0011546082,0.000018242683,0.000001750652,0.0000014385894,0.00019530216,0.000027755477,0.00090826146],"genre_scores_gemma":[0.9987649,0.00011542993,0.00067572616,0.0000031892932,0.000011334568,0.000001890138,0.00034653064,0.0000056314216,0.00007552802],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994516,0.000012824489,0.0000050314325,0.00001687951,0.000012393133,0.0000077829645],"domain_scores_gemma":[0.9994112,0.00013530259,0.0002978706,0.00006522883,0.000047278085,0.000043163935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017961084,0.00020615813,0.00018640999,0.0012552112,0.000087092514,0.00035292143,0.00017140932,0.000113336035,0.00057870866],"category_scores_gemma":[0.0009467973,0.000086830216,0.00019561611,0.0009194157,0.00016485389,0.0003217358,0.00031942734,0.00014904611,0.00014062096],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010201375,0.000015921136,0.9496576,0.000048185815,0.000093965304,0.000069019305,0.00045232315,0.0052433885,0.010060329,0.0005977086,0.00026811505,0.03339132],"study_design_scores_gemma":[0.000005087447,0.00002451518,0.9956964,0.0000045331485,0.000017104776,0.00003974367,0.000060204562,0.002681294,0.0004928008,0.00015871957,0.000813496,0.0000059916306],"about_ca_topic_score_codex":0.0033658925,"about_ca_topic_score_gemma":0.006332711,"teacher_disagreement_score":0.0033658925,"about_ca_system_score_codex":0.0001934718,"about_ca_system_score_gemma":0.00010368333,"threshold_uncertainty_score":0.006692648},"labels":[],"label_agreement":null},{"id":"W1989560122","doi":"10.1086/528932","title":"The Total Merger Rate of Compact Object Binaries in the Local Universe","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Neutron star; LIGO; Astrophysics; Black hole (networking); Compact star; Gravitational wave; Stellar black hole; Population; Astronomy; Universe; Binary black hole; Star cluster; Stars; Galaxy","score_opus":0.01390115290714729,"score_gpt":0.28994872351166573,"score_spread":0.27604757060451846,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989560122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975573,0.000069594695,0.0015020116,0.000011020021,8.840318e-7,0.000004343045,0.00016622916,0.00003003883,0.0006586427],"genre_scores_gemma":[0.99831164,0.000063817875,0.00091372273,0.000004573661,0.0000029312887,0.0000067435167,0.00038717355,0.000010313276,0.0002990267],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998988,0.000025449519,0.00000620207,0.00003640257,0.000016195128,0.000016981512],"domain_scores_gemma":[0.9993012,0.00025151385,0.00019944008,0.000072353265,0.00007524805,0.00010028085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054209994,0.0002521663,0.00028987828,0.00091903115,0.00020210804,0.00085852545,0.00031963998,0.00026844445,0.0011489973],"category_scores_gemma":[0.0025406193,0.00019391635,0.00041217628,0.000555976,0.00028557266,0.00049914734,0.0005485412,0.00018983377,0.00020778798],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034835818,0.00007212496,0.6963352,0.00008572267,0.00031824998,0.00034023702,0.0005489297,0.26193553,0.010401741,0.008939444,0.00039253396,0.020281918],"study_design_scores_gemma":[0.000039840732,0.00013553066,0.33786184,0.000012349289,0.00015933179,0.0004383139,0.00023522145,0.65052277,0.00603714,0.003677997,0.00083999115,0.000039797065],"about_ca_topic_score_codex":0.005115345,"about_ca_topic_score_gemma":0.0033570875,"teacher_disagreement_score":0.005115345,"about_ca_system_score_codex":0.000546483,"about_ca_system_score_gemma":0.00017670909,"threshold_uncertainty_score":0.010171115},"labels":[],"label_agreement":null},{"id":"W1989643238","doi":"10.1086/511262","title":"Observations of the Unidentified TeV γ‐Ray Source TeV J2032+4130 with the Whipple Observatory 10 m Telescope","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Observatory; Telescope; Sky; Astrophysics; Flux (metallurgy); Crab Nebula; Astronomy; Nebula; Gamma ray; Stars","score_opus":0.015594033138620783,"score_gpt":0.21542990194339193,"score_spread":0.19983586880477114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989643238","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99722326,0.00029001408,0.00040690793,0.000038588896,0.0000073293586,0.000016420048,0.0005796439,0.00003670311,0.001401154],"genre_scores_gemma":[0.9932114,0.00043478017,0.0022042384,0.0000988247,0.000023865181,0.000021127758,0.0027588545,0.000023988126,0.0012228165],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980956,0.0000142450735,0.000009768383,0.00004785422,0.00006711826,0.000051534043],"domain_scores_gemma":[0.9995764,0.000037725822,0.0001966497,0.000062865845,0.000025603318,0.000100784455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026779514,0.00037721172,0.0003957964,0.00091619015,0.0007478067,0.00057885953,0.00045110978,0.00047327986,0.0009516408],"category_scores_gemma":[0.0003111618,0.00029803487,0.00033851922,0.0012814233,0.00020331993,0.0003358584,0.00080816867,0.0005624973,0.00041304925],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001053833,0.00026477914,0.6801188,0.00021427197,0.00021626787,0.014538306,0.0020975508,0.0017050885,0.26014125,0.000781559,0.003338145,0.035530116],"study_design_scores_gemma":[0.000023843777,0.00014831542,0.9893063,0.000023793486,0.000027096827,0.0020391075,0.00014642681,0.00045320892,0.0039380486,0.00014155729,0.0037234593,0.000028836283],"about_ca_topic_score_codex":0.0050346754,"about_ca_topic_score_gemma":0.022615531,"teacher_disagreement_score":0.0050346754,"about_ca_system_score_codex":0.00037937282,"about_ca_system_score_gemma":0.00033941554,"threshold_uncertainty_score":0.010010779},"labels":[],"label_agreement":null},{"id":"W1989649987","doi":"10.1086/589765","title":"The Size Function of Galaxy Disks out to<i>z</i>∼ 1 from the Canada‐France‐Hawaii‐Telescope Legacy Survey","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Redshift; Physics; Galaxy; Luminosity function; Luminosity; Galaxy formation and evolution; Sky; Astronomy; Universe; Cosmic variance","score_opus":0.011095736714459063,"score_gpt":0.20440989611164836,"score_spread":0.1933141593971893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989649987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.908167,0.0019040396,0.00023017578,0.0006441289,0.00005403099,0.000021206191,0.07986246,0.00017319093,0.008943787],"genre_scores_gemma":[0.92451644,0.00080933707,0.00022155837,0.00019950459,0.00006737163,0.00001975131,0.067073174,0.000056162567,0.0070367777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998324,0.0000073736464,0.000006464498,0.00004662369,0.00005051449,0.000056599827],"domain_scores_gemma":[0.9966754,0.00031382914,0.00060701004,0.00016478643,0.0013558473,0.00088312273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003929242,0.00025886783,0.00026629577,0.0028277135,0.00046152226,0.00070324657,0.0006917792,0.00041907362,0.003416542],"category_scores_gemma":[0.0019461744,0.0002554515,0.00027553356,0.001741966,0.0002784793,0.00044237805,0.00048262152,0.0003561567,0.0012615409],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009767775,0.000015390326,0.9563462,0.000101676174,0.000094760326,0.00008584501,0.00048978877,0.0006478528,0.0016421624,0.00043820115,0.029005801,0.011034682],"study_design_scores_gemma":[0.0000015259058,0.0000017585862,0.99786335,0.000003955144,0.000006061481,0.000009962594,0.00003699993,0.000053908356,0.000047264228,0.000014991927,0.001957932,0.000002360047],"about_ca_topic_score_codex":0.42531368,"about_ca_topic_score_gemma":0.5257263,"teacher_disagreement_score":0.42531368,"about_ca_system_score_codex":0.0016173165,"about_ca_system_score_gemma":0.0016070007,"threshold_uncertainty_score":0.8456762},"labels":[],"label_agreement":null},{"id":"W1989689287","doi":"10.1086/592061","title":"Electrodynamics of Magnetars. IV. Self‐Consistent Model of the Inner Accelerator with Implications for Pulsed Radio Emission","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Magnetar; Pulsar; Magnetic field; Magnetosphere; Scattering; Polar; Radio frequency; Photon; Voltage","score_opus":0.01739875668636356,"score_gpt":0.27888872518394087,"score_spread":0.26148996849757733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989689287","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6810992,0.002540166,0.18466128,0.0042622904,0.00044335707,0.00015227469,0.00034699513,0.0005712968,0.12592308],"genre_scores_gemma":[0.97283787,0.0004119743,0.0073948423,0.00038674838,0.000115545394,0.00011426397,0.00007484928,0.00008089573,0.018582975],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998901,0.00003159984,0.000004459657,0.000014436933,0.00003226833,0.000027176518],"domain_scores_gemma":[0.99985266,0.00003048921,0.000027879842,0.00002230813,0.000033954155,0.00003262992],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000313953,0.00033606193,0.00048731518,0.00037522946,0.0007321471,0.0010598081,0.0011695096,0.0010661853,0.00253511],"category_scores_gemma":[0.00041619185,0.0002801789,0.00063458463,0.00026115298,0.0013379266,0.0011431425,0.000858251,0.0006459262,0.0005467046],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010241803,0.000100183,0.0026590044,0.00005850917,0.00004354435,0.0005119075,0.00029443693,0.39587554,0.0131372735,0.5790766,0.0032217493,0.0049188887],"study_design_scores_gemma":[0.00005086789,0.0000968716,0.0015955389,0.000010254347,0.0000101467185,0.00015855799,0.000097198725,0.8990838,0.00072123995,0.09551095,0.0026415747,0.000023086326],"about_ca_topic_score_codex":0.0021590998,"about_ca_topic_score_gemma":0.0009975182,"teacher_disagreement_score":0.00253511,"about_ca_system_score_codex":0.0010639577,"about_ca_system_score_gemma":0.0005905227,"threshold_uncertainty_score":0.008480787},"labels":[],"label_agreement":null},{"id":"W1989731716","doi":"10.1088/0004-637x/726/1/56","title":"MULTI-EPOCH ANALYSIS OF PULSE SHAPES FROM THE NEUTRON STAR SAX J1808.4–3658","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; University of Alberta","funders":"","keywords":"RADIUS; Neutron star; Sigma; Confidence region; Star (game theory); Pulse (music); Hadron","score_opus":0.013876799868127659,"score_gpt":0.3151133237018383,"score_spread":0.30123652383371063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989731716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99777055,0.00007431294,0.0011911646,0.00002164747,0.0000064743226,0.0000057670427,0.000358832,0.000055490287,0.0005158916],"genre_scores_gemma":[0.9970285,0.000058897756,0.0014381038,0.000007625197,0.00001140885,0.000006037063,0.0011473707,0.000027263086,0.0002747829],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.000016480157,0.0000102750455,0.000036146885,0.00004069176,0.000018708544],"domain_scores_gemma":[0.9991284,0.00027123452,0.00027485474,0.0001037515,0.00009910277,0.00012266326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005588828,0.0004042716,0.0003960493,0.0023260643,0.0003585111,0.0005138213,0.0002971352,0.0003752951,0.0007700444],"category_scores_gemma":[0.0010160679,0.00033001677,0.0005684851,0.0012863189,0.00017197987,0.0003235537,0.0005122606,0.00046232739,0.00021471283],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016236692,0.0002574752,0.7636627,0.0002183589,0.00045410622,0.0017687407,0.0010480636,0.022800755,0.15180224,0.0010571242,0.0007972411,0.054509535],"study_design_scores_gemma":[0.00002017091,0.0001501611,0.958664,0.000013524658,0.00011178869,0.0007969997,0.00012688997,0.03047479,0.008290461,0.00023993936,0.0010727785,0.00003853287],"about_ca_topic_score_codex":0.0015271411,"about_ca_topic_score_gemma":0.0032338921,"teacher_disagreement_score":0.0023260643,"about_ca_system_score_codex":0.0003070532,"about_ca_system_score_gemma":0.00016201027,"threshold_uncertainty_score":0.003036499},"labels":[],"label_agreement":null},{"id":"W1989738732","doi":"10.1086/308392","title":"Tidally Triggered Star Formation in Close Pairs of Galaxies","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":355,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Astrophysics; Physics; Redshift; Star formation; Spectral line; Astronomy; Sample (material); Galaxy formation and evolution","score_opus":0.006852667808122915,"score_gpt":0.20461321177411115,"score_spread":0.19776054396598824,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989738732","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996861,0.000039348815,0.000059308502,0.00000369981,7.7228884e-7,0.0000014828547,0.00011012224,0.0000040689183,0.00009508951],"genre_scores_gemma":[0.99922264,0.000015814323,0.000092335526,0.000002813472,0.0000034304455,0.0000027115584,0.00059656287,0.0000014470806,0.00006226933],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996617,0.00006750476,0.000022533359,0.00011649392,0.000066161614,0.00006567579],"domain_scores_gemma":[0.9983979,0.00032154992,0.0006032937,0.00023312899,0.00011708908,0.00032697324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034503767,0.00023892571,0.00038290906,0.0017904183,0.00040467374,0.00059886597,0.00034778882,0.00029555248,0.0008359772],"category_scores_gemma":[0.0015207336,0.00021914158,0.000276337,0.0013841558,0.00034804686,0.00046126256,0.00061792287,0.00018023806,0.0002480595],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000201379,0.00006480263,0.989603,0.000014715333,0.000089208894,0.00020338122,0.00039746598,0.00030910302,0.0058018314,0.000071879265,0.0001301487,0.003113119],"study_design_scores_gemma":[0.0000039235983,0.000033084292,0.99845266,0.0000014839644,0.000013450717,0.00020253043,0.00013800658,0.0006081133,0.00034055233,0.000025210331,0.00017813129,0.0000029092514],"about_ca_topic_score_codex":0.0026834346,"about_ca_topic_score_gemma":0.0040406077,"teacher_disagreement_score":0.0026834346,"about_ca_system_score_codex":0.00025170317,"about_ca_system_score_gemma":0.000070560774,"threshold_uncertainty_score":0.0053356886},"labels":[],"label_agreement":null},{"id":"W1989763959","doi":"10.1086/309530","title":"The MACHO Project Large Magellanic Cloud Variable‐Star Inventory. IX. Frequency Analysis of the First‐Overtone RR Lyrae Stars and the Indication for Nonradial Pulsations","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Toronto","funders":"","keywords":"RR Lyrae variable; Overtone; Astrophysics; Large Magellanic Cloud; Variable star; Physics; Stars; Population; Spectral line; Astronomy; Globular cluster","score_opus":0.008190163024742078,"score_gpt":0.22737338066717716,"score_spread":0.2191832176424351,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989763959","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.06745663,0.0012207889,0.0027699596,0.0012101566,0.00012264549,0.00028343656,0.8952782,0.0038435042,0.027814686],"genre_scores_gemma":[0.115572974,0.00055903674,0.014023156,0.0002444982,0.00013576874,0.00049687485,0.8533994,0.00058491726,0.014983323],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9995233,0.000043521995,0.000047314916,0.00006346282,0.00024302232,0.00007941081],"domain_scores_gemma":[0.99729055,0.00015404439,0.00063920784,0.0003349601,0.0010458687,0.0005353678],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011485586,0.00066615356,0.00063181226,0.0056797205,0.0007150249,0.0015088458,0.0014479237,0.00043964866,0.008328683],"category_scores_gemma":[0.003255413,0.0004237302,0.00036501905,0.0045450716,0.0002002287,0.0015096241,0.0024684137,0.00052965234,0.005376063],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016136958,0.00037441787,0.26718363,0.0007290445,0.00024891028,0.00026338286,0.0005191579,0.0011588946,0.0040265406,0.004338968,0.5614708,0.1580726],"study_design_scores_gemma":[0.00042927658,0.00012258938,0.62003356,0.00016845578,0.000144944,0.0001598187,0.00039614327,0.004669311,0.0038773054,0.002175773,0.36776865,0.00005415057],"about_ca_topic_score_codex":0.08635837,"about_ca_topic_score_gemma":0.081471324,"teacher_disagreement_score":0.08635837,"about_ca_system_score_codex":0.0012589367,"about_ca_system_score_gemma":0.002106079,"threshold_uncertainty_score":0.17171139},"labels":[],"label_agreement":null},{"id":"W1989821526","doi":"10.1086/338386","title":"Globular Cluster Systems in Four Brightest Cluster Galaxies: A262, A3560, A3565, and A3742","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Globular cluster; Brightest cluster galaxy; Galaxy cluster; Cluster (spacecraft); Astrophysics; Astronomy; Open cluster; Galaxy; Galaxy groups and clusters; Star cluster; Stars","score_opus":0.009151098086184015,"score_gpt":0.19696844838375432,"score_spread":0.1878173502975703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989821526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99977463,0.000017688297,0.000016053164,0.000001976831,3.6940676e-7,0.0000012249035,0.000050654457,0.000002344871,0.00013508757],"genre_scores_gemma":[0.9991177,0.000016270496,0.00014746762,0.000008424472,0.0000015056756,0.0000016780951,0.0004984808,0.0000014838402,0.00020706144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998022,0.000017046492,0.000011679235,0.00006394748,0.00003551564,0.00006970935],"domain_scores_gemma":[0.9996941,0.000017029342,0.000064414664,0.000038249796,0.00004249902,0.00014362023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021581624,0.00033706252,0.00021872827,0.0012096518,0.00072278816,0.0004467868,0.00020719723,0.00020953138,0.0010113174],"category_scores_gemma":[0.00037349339,0.00018700639,0.00021182233,0.0007255421,0.00034133033,0.00030237576,0.0005577873,0.00016236334,0.00028593827],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001931896,0.00010263001,0.96664256,0.000019156729,0.000060370592,0.00031876191,0.0012903828,0.00046685277,0.025091525,0.0003444711,0.0002855503,0.005184555],"study_design_scores_gemma":[0.000012328647,0.000068982394,0.9979233,0.0000021654098,0.000013407301,0.00018640458,0.00021957481,0.00027752356,0.0007058851,0.0000649403,0.0005207695,0.000004687028],"about_ca_topic_score_codex":0.026375337,"about_ca_topic_score_gemma":0.04209911,"teacher_disagreement_score":0.026375337,"about_ca_system_score_codex":0.000542815,"about_ca_system_score_gemma":0.00019818758,"threshold_uncertainty_score":0.052443624},"labels":[],"label_agreement":null},{"id":"W1989871154","doi":"10.1086/378316","title":"Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. II. The Fine Structure of Simulated Galactic Disks","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":581,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Stars; Thick disk; Accretion (finance); Galaxy; Thin disk; Cold dark matter; Population; Surface brightness; Debris disk","score_opus":0.006201563116525914,"score_gpt":0.20960244061918912,"score_spread":0.2034008775026632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989871154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99168044,0.00015537399,0.0030900694,0.00018863057,0.000017734328,0.000042798238,0.0009585181,0.00013733927,0.0037290044],"genre_scores_gemma":[0.9938309,0.000116123,0.0038909044,0.000077442,0.000011028366,0.000074871474,0.0009188833,0.000034088338,0.0010456798],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998555,0.00004880333,0.000008092022,0.000023137174,0.000021634773,0.00004269146],"domain_scores_gemma":[0.9989492,0.000510654,0.00012895936,0.00008173886,0.00013775233,0.00019169334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043007365,0.00044801485,0.0004606678,0.0005996219,0.00054183905,0.0006785341,0.001238359,0.0009822573,0.002148722],"category_scores_gemma":[0.0020266918,0.00037063402,0.0005403228,0.0006294214,0.0005674844,0.00056577346,0.00078377855,0.00071303215,0.0002195061],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025649316,0.00013318205,0.024365986,0.00004245532,0.00006878349,0.000134493,0.00015158288,0.96814716,0.00096064573,0.0035804398,0.0005463316,0.0016124907],"study_design_scores_gemma":[0.000068428584,0.000051665265,0.0037699775,0.000008147664,0.000011762986,0.000019998144,0.00006596829,0.9940316,0.00023788222,0.001310949,0.0004158044,0.000007726312],"about_ca_topic_score_codex":0.033816084,"about_ca_topic_score_gemma":0.0223857,"teacher_disagreement_score":0.033816084,"about_ca_system_score_codex":0.0013933716,"about_ca_system_score_gemma":0.00057358795,"threshold_uncertainty_score":0.06723851},"labels":[],"label_agreement":null},{"id":"W1989886558","doi":"10.1088/0004-637x/770/1/30","title":"ACCRETION DISK TEMPERATURES OF QSOs: CONSTRAINTS FROM THE EMISSION LINES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Quest University Canada","funders":"Los Alamos National Laboratory; Fermilab; Max-Planck-Institut für Astronomie; University of Pittsburgh; Johns Hopkins University; Max-Planck-Gesellschaft; New Mexico State University; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Astrophysics; QSOS; Physics; Accretion (finance); Emission spectrum; Accretion disc; Spectral line; Intermediate polar; Thin disk; Ionization; Line (geometry); Astronomy; Quasar; Galaxy; Stars; White dwarf","score_opus":0.010481953527573768,"score_gpt":0.23017878001841605,"score_spread":0.21969682649084227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989886558","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881893,0.00016951618,0.00035231892,0.000013286591,0.0000017115115,0.0000025059367,0.00014226545,0.000008456246,0.0004909857],"genre_scores_gemma":[0.9996674,0.000047130325,0.000098076765,0.00000307699,0.00000610392,0.0000018364524,0.00014033729,0.000003986188,0.000032022905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989057,0.000017944185,0.000008791154,0.000036081936,0.000022872606,0.000023684359],"domain_scores_gemma":[0.9991636,0.00032534424,0.0002810662,0.0000560683,0.00007535028,0.00009851759],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026288343,0.00030143544,0.0002772485,0.00080334337,0.00022519808,0.0007338536,0.0003090264,0.00033977034,0.000756363],"category_scores_gemma":[0.0018060749,0.00020564375,0.00015641966,0.00043816795,0.0003463307,0.0005295272,0.00034750346,0.00019458462,0.00028799157],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009204772,0.00009661207,0.8913336,0.00011078424,0.000092369344,0.00040745706,0.0005452474,0.0059340484,0.091352135,0.0010036197,0.00020754997,0.007996112],"study_design_scores_gemma":[0.000035832756,0.00010468316,0.9776464,0.000012804741,0.000035310342,0.00022833984,0.00014559024,0.012690218,0.008070822,0.0007249318,0.0002885666,0.0000165548],"about_ca_topic_score_codex":0.0016147414,"about_ca_topic_score_gemma":0.001288023,"teacher_disagreement_score":0.0016147414,"about_ca_system_score_codex":0.000351635,"about_ca_system_score_gemma":0.00010772519,"threshold_uncertainty_score":0.0032107234},"labels":[],"label_agreement":null},{"id":"W1989936011","doi":"10.1086/308741","title":"The Ionization Source in the Nucleus of M84","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Point source; Galaxy; Astronomy; Spectral energy distribution; Luminosity; Doubly ionized oxygen; Supermassive black hole; Space Telescope Imaging Spectrograph; Hubble Deep Field South; Spitzer Space Telescope; Stars; Emission spectrum; Spectral line; Hubble Deep Field; Redshift; Hubble space telescope; Optics","score_opus":0.004733204460083074,"score_gpt":0.19521214421255587,"score_spread":0.1904789397524728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1989936011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99236476,0.0002571782,0.0004506431,0.00008030789,0.000014898399,0.000005497944,0.00027973994,0.000037588256,0.006509427],"genre_scores_gemma":[0.99536824,0.0001618694,0.0011457419,0.000055378285,0.00002671873,0.00000777371,0.0009662244,0.000014215566,0.0022539073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998721,0.000008568894,0.0000046002924,0.000030399942,0.000045612007,0.000038626476],"domain_scores_gemma":[0.9997434,0.000017821592,0.00009461596,0.000043861208,0.000041838928,0.000058417143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015443581,0.00017682942,0.00027545844,0.00081909646,0.0011822894,0.00045210545,0.00042297377,0.0003772216,0.0031003614],"category_scores_gemma":[0.0005768135,0.00015867525,0.00013533044,0.00085251906,0.0003414638,0.00043423442,0.0018360295,0.00040642254,0.0016882594],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005868143,0.00021796404,0.7285733,0.00018883015,0.000059699367,0.003195422,0.0037078913,0.0008512605,0.19576038,0.0036883438,0.0047891494,0.058380947],"study_design_scores_gemma":[0.000032224714,0.00017666961,0.964143,0.000051565763,0.00002343725,0.0019112964,0.0006535417,0.0008677318,0.0067076534,0.0014044954,0.024010362,0.000018047162],"about_ca_topic_score_codex":0.002568541,"about_ca_topic_score_gemma":0.0037277143,"teacher_disagreement_score":0.0031003614,"about_ca_system_score_codex":0.0005022855,"about_ca_system_score_gemma":0.00020409841,"threshold_uncertainty_score":0.010371745},"labels":[],"label_agreement":null},{"id":"W1990088268","doi":"10.1088/0004-637x/723/1/649","title":"<i>FERMI</i>LARGE AREA TELESCOPE OBSERVATION OF A GAMMA-RAY SOURCE AT THE POSITION OF ETA CARINAE","year":2010,"lang":"ru","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Fermi Gamma-ray Space Telescope; Telescope; Astrophysics; Flare; Flux (metallurgy); Spitzer Space Telescope; Gamma ray; Light curve; Astronomy; Photon; Optics","score_opus":0.009424859459816599,"score_gpt":0.2137592547898612,"score_spread":0.2043343953300446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990088268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7955356,0.0035839577,0.009840946,0.00979985,0.001829777,0.00015800695,0.04922669,0.0022078985,0.12781735],"genre_scores_gemma":[0.9569266,0.0007592599,0.012308847,0.0013153454,0.0005998784,0.00003667859,0.017922966,0.00018184209,0.009948501],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998747,0.0000065721965,0.000007743083,0.000030144496,0.00005003243,0.00003072011],"domain_scores_gemma":[0.99966884,0.000036578338,0.000116167255,0.000047288147,0.0000788995,0.000052230815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020922115,0.00027331695,0.00020465048,0.0015485414,0.0007722452,0.0005104922,0.00048005852,0.0006333949,0.008936236],"category_scores_gemma":[0.00038011963,0.000119881406,0.00020945448,0.0010060597,0.00034885207,0.00038753854,0.00048463955,0.0004148627,0.0010715756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009867181,0.00024271273,0.3936044,0.00072528113,0.0002858579,0.007913514,0.0014763317,0.0017804563,0.16504388,0.0080025485,0.31036618,0.10957205],"study_design_scores_gemma":[0.00003392374,0.00010761785,0.7910303,0.00015314891,0.00005571519,0.004155639,0.00036520275,0.0022525445,0.01898505,0.001491507,0.18130365,0.00006559683],"about_ca_topic_score_codex":0.009562461,"about_ca_topic_score_gemma":0.030469893,"teacher_disagreement_score":0.009562461,"about_ca_system_score_codex":0.0006829472,"about_ca_system_score_gemma":0.0002881734,"threshold_uncertainty_score":0.02989465},"labels":[],"label_agreement":null},{"id":"W1990130516","doi":"10.1086/338799","title":"A Phase-connected Timing Solution for the Magnetar Candidate 1E 1841−045","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Magnetar; Pulsar; Astrophysics; Ephemeris; Flux (metallurgy); Astronomy; Supernova; Accretion (finance); Noise (video); Binary pulsar; Phase (matter); Millisecond pulsar; Supernova remnant; X-ray pulsar; Satellite","score_opus":0.029993806969162554,"score_gpt":0.32691870954840185,"score_spread":0.2969249025792393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990130516","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93891096,0.00015107892,0.055528015,0.00026059648,0.00006498697,0.00003129755,0.00048819502,0.00022794533,0.00433694],"genre_scores_gemma":[0.9570051,0.00007316578,0.040709313,0.000029512914,0.000059709564,0.00002027513,0.001152804,0.00003523059,0.00091497885],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99994445,0.000009457261,0.000004206001,0.000020005027,0.000013367537,0.000008544037],"domain_scores_gemma":[0.9997414,0.000047671812,0.00011090278,0.000023707626,0.00004083614,0.000035458015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016236132,0.00022393331,0.00014180658,0.00065959356,0.0002703152,0.00045725246,0.000361563,0.00039800018,0.0018620844],"category_scores_gemma":[0.0015062038,0.00012963812,0.00016727351,0.0005356215,0.00013732347,0.00024975228,0.00030691214,0.00029205225,0.00032288162],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010933981,0.00027403884,0.23445661,0.0002937959,0.00020060941,0.0032317715,0.00072828616,0.25681183,0.08967142,0.050224483,0.0066587017,0.3563551],"study_design_scores_gemma":[0.000411723,0.0006394783,0.21745224,0.000048668924,0.00014277715,0.0019070661,0.00032084875,0.71242195,0.014979212,0.031393368,0.020183662,0.00009898348],"about_ca_topic_score_codex":0.0011254605,"about_ca_topic_score_gemma":0.0026188153,"teacher_disagreement_score":0.0018620844,"about_ca_system_score_codex":0.00018430401,"about_ca_system_score_gemma":0.00038063512,"threshold_uncertainty_score":0.0062292814},"labels":[],"label_agreement":null},{"id":"W1990261454","doi":"10.1088/0004-637x/729/2/142","title":"INTRACLUSTER SUPERNOVAE IN THE MULTI-EPOCH NEARBY CLUSTER SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Astrophysics; Physics; Astronomy; Galaxy cluster; Supernova; Galaxy; Population; Intracluster medium; Cluster (spacecraft); Type-cD galaxy; Brightest cluster galaxy; Medicine","score_opus":0.037219805618565936,"score_gpt":0.25314421693921596,"score_spread":0.21592441132065002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990261454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99526334,0.00041144658,0.0008260721,0.000045279652,0.000012863158,0.000014945935,0.0009830922,0.000047899426,0.0023950506],"genre_scores_gemma":[0.9974286,0.00014424205,0.0006003485,0.00001684249,0.000009349652,0.0000068491763,0.0013544156,0.000008549322,0.00043078634],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996722,0.00004285862,0.000031339656,0.00009084962,0.000109109526,0.0000535744],"domain_scores_gemma":[0.99905676,0.00011031088,0.00039506028,0.000121140205,0.00012840024,0.00018838262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005528089,0.00019486719,0.00021644087,0.0012274898,0.00031619324,0.0004003923,0.00037483565,0.00023899792,0.0009795313],"category_scores_gemma":[0.001705819,0.00012833023,0.00043213894,0.0009255855,0.00015937716,0.00023909344,0.00075531495,0.00021572798,0.00024325002],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022402344,0.000005381626,0.9945852,0.000010869711,0.00005606633,0.000057649846,0.000039274953,0.000853291,0.0004115026,0.00028026724,0.0003242048,0.003353899],"study_design_scores_gemma":[0.0000016202052,0.00001077222,0.99750227,0.0000071106188,0.00001805453,0.000104828934,0.000019128838,0.0011719711,0.0001268198,0.00007679088,0.00095852115,0.000002049218],"about_ca_topic_score_codex":0.025292192,"about_ca_topic_score_gemma":0.030191131,"teacher_disagreement_score":0.025292192,"about_ca_system_score_codex":0.00050021976,"about_ca_system_score_gemma":0.0002938605,"threshold_uncertainty_score":0.05028993},"labels":[],"label_agreement":null},{"id":"W1990611595","doi":"10.1086/322346","title":"Dynamics of the Globular Cluster System Associated with M87 (NGC 4486). I. New CFHT MOS Spectroscopy and the Composite Database","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; Queen's University; University of Waterloo; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Observatory; Astrophysics; Photometry (optics); Astronomy; Galaxy; Telescope; Star cluster; Virgo Cluster; Spectrograph; Galaxy cluster; Database; Spectral line; Stars; Computer science","score_opus":0.004000256485964563,"score_gpt":0.19083363221332583,"score_spread":0.18683337572736128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990611595","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9085479,0.0005584494,0.00032082203,0.000066128385,0.0000058699165,0.00003426749,0.087013215,0.000104456085,0.003348869],"genre_scores_gemma":[0.83280814,0.0006906206,0.0012535279,0.00003040873,0.000023472332,0.000042989523,0.16391349,0.000021221547,0.0012162767],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999723,0.000016483295,0.000030491656,0.000079294914,0.00010330275,0.0000473937],"domain_scores_gemma":[0.9989743,0.00008393598,0.00042665086,0.00014771993,0.0002195197,0.00014789472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020696563,0.00023291323,0.0002913984,0.0038201062,0.0003195227,0.000600028,0.00033320984,0.0002146811,0.0016397287],"category_scores_gemma":[0.0009473866,0.000108199674,0.00018908335,0.0032229084,0.00015774369,0.0004279734,0.0006276686,0.0001568987,0.0007107517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015695287,0.000069047965,0.9603877,0.000111999834,0.00006753427,0.00016715945,0.00031821034,0.0013139071,0.002264028,0.000710071,0.0069220252,0.027511531],"study_design_scores_gemma":[0.0000026146527,0.000014337372,0.993472,0.0000069851717,0.000012675417,0.000091386144,0.000058753576,0.00104612,0.00036048584,0.000076748904,0.004853584,0.0000043568925],"about_ca_topic_score_codex":0.04817537,"about_ca_topic_score_gemma":0.059870347,"teacher_disagreement_score":0.04817537,"about_ca_system_score_codex":0.00080456375,"about_ca_system_score_gemma":0.00037627865,"threshold_uncertainty_score":0.09578991},"labels":[],"label_agreement":null},{"id":"W1990620438","doi":"10.1088/0004-637x/700/2/l123","title":"NO NEUTRON STAR COMPANION TO THE LOWEST MASS SDSS WHITE DWARF","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Associated Universities; National Aeronautics and Space Administration","keywords":"White dwarf; Physics; Neutron star; Pulsar; Astrophysics; Millisecond pulsar; Astronomy; Radio telescope; Telescope; Compact star; Stars","score_opus":0.011292948902459517,"score_gpt":0.23019115495460374,"score_spread":0.21889820605214422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990620438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99180204,0.00021873653,0.00024655327,0.00006704099,0.00004856908,0.000015705864,0.0009023989,0.000033053897,0.006665956],"genre_scores_gemma":[0.9936651,0.00014715234,0.00035481117,0.00009425719,0.000024810417,0.000009281318,0.0021549766,0.000010664225,0.0035390754],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982363,0.000009355652,0.000022095266,0.000054363034,0.000057761685,0.000032865442],"domain_scores_gemma":[0.9991134,0.00010443072,0.00031983393,0.00011599713,0.00009518097,0.00025120075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017217232,0.00015418479,0.00028105968,0.00037502008,0.0006750855,0.00048275263,0.00022511263,0.00027792866,0.0071221567],"category_scores_gemma":[0.00088378834,0.00011968871,0.00011726749,0.00032973906,0.00024020688,0.00026780204,0.000498045,0.00020692262,0.0017521366],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006400544,0.00017638432,0.9043401,0.00028104347,0.000080499805,0.0041995593,0.0009512767,0.00008363634,0.059665613,0.0012905125,0.003087049,0.025204267],"study_design_scores_gemma":[0.000033516484,0.00050249376,0.8900458,0.000049019993,0.00006433222,0.015937185,0.00070544006,0.00029501217,0.016198345,0.0006760751,0.075469404,0.000023323732],"about_ca_topic_score_codex":0.0020135255,"about_ca_topic_score_gemma":0.0033169675,"teacher_disagreement_score":0.0071221567,"about_ca_system_score_codex":0.0003035893,"about_ca_system_score_gemma":0.00031752212,"threshold_uncertainty_score":0.023826003},"labels":[],"label_agreement":null},{"id":"W1990795959","doi":"10.1088/0004-637x/726/2/92","title":"DISCOVERY OF A NEW AM CVn SYSTEM WITH THE<i>KEPLER</i>SATELLITE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science Mission Directorate; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Centre National d’Etudes Spatiales; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Light curve; Astrophysics; Photometry (optics); Astronomy; Accretion (finance); Stars; Gravitational microlensing; Spectral line","score_opus":0.0067395478997584165,"score_gpt":0.21162235633838747,"score_spread":0.20488280843862905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990795959","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8895384,0.0013580491,0.008175647,0.0027186675,0.0009753733,0.00018827502,0.00090252806,0.00047640194,0.095666625],"genre_scores_gemma":[0.9788946,0.0001487273,0.01045219,0.00077079324,0.00015614489,0.00005233561,0.00079020124,0.000082251194,0.008652812],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9995695,0.000044524804,0.000009705705,0.00018936879,0.0001003579,0.00008667256],"domain_scores_gemma":[0.9992686,0.000089431116,0.000081307226,0.00012746634,0.00013829242,0.00029484296],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001128144,0.00030849333,0.00042002412,0.00065920077,0.001326841,0.0021418282,0.000795532,0.0014911501,0.0029615657],"category_scores_gemma":[0.0013842626,0.00036730475,0.00043326398,0.00068994315,0.00074451906,0.0010110321,0.002236846,0.0013363513,0.0008135247],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00232374,0.0005916437,0.14449774,0.0006777948,0.00050764566,0.0070656817,0.0024566955,0.0030358427,0.5819235,0.08645157,0.026732292,0.14373592],"study_design_scores_gemma":[0.0018439222,0.0042143087,0.46659052,0.00046497377,0.00083109475,0.007865163,0.0016089465,0.028714433,0.1220607,0.02735339,0.33808535,0.00036719468],"about_ca_topic_score_codex":0.0024995178,"about_ca_topic_score_gemma":0.0029489023,"teacher_disagreement_score":0.0029615657,"about_ca_system_score_codex":0.0012097239,"about_ca_system_score_gemma":0.0009935432,"threshold_uncertainty_score":0.009907484},"labels":[],"label_agreement":null},{"id":"W1990805180","doi":"10.1086/500252","title":"Testing Rotational Mixing Predictions with New Boron Abundances in Main‐Sequence B‐Type Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Stars; Boron; Astrophysics; Physics; Mixing (physics); Abundance (ecology); Spectral line; Rotation (mathematics); Stellar evolution; Astronomy; Geometry","score_opus":0.01764750048739761,"score_gpt":0.23331141863519322,"score_spread":0.21566391814779562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990805180","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98942953,0.00009747671,0.007410434,0.00018065536,0.00004775077,0.000037753907,0.00077032845,0.00016284845,0.0018632209],"genre_scores_gemma":[0.99652356,0.00003754713,0.0021901508,0.00009174478,0.000009926245,0.000020410109,0.0007783932,0.0000577269,0.00029044118],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993795,0.00016544576,0.000042635544,0.0002289003,0.000119857825,0.00006362428],"domain_scores_gemma":[0.99777216,0.001282538,0.0002528253,0.0002606648,0.00025466998,0.00017708943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032979958,0.0008949191,0.00048028308,0.00037830128,0.00090378296,0.0011242968,0.0010705461,0.0011015434,0.004600936],"category_scores_gemma":[0.004265473,0.00040039423,0.0009539147,0.00025110634,0.0007433801,0.0013023801,0.00080427714,0.0007277736,0.001370997],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.02100609,0.001514647,0.5353342,0.00038697035,0.00087272964,0.00031755754,0.00039414453,0.048375946,0.3564221,0.004418137,0.001549741,0.02940767],"study_design_scores_gemma":[0.0036064163,0.0069657494,0.25777644,0.00009331641,0.0012293364,0.0003330012,0.0005941973,0.33374694,0.37764245,0.013482528,0.004367746,0.00016187956],"about_ca_topic_score_codex":0.0057930383,"about_ca_topic_score_gemma":0.004341636,"teacher_disagreement_score":0.0057930383,"about_ca_system_score_codex":0.00077228976,"about_ca_system_score_gemma":0.0005096649,"threshold_uncertainty_score":0.01744169},"labels":[],"label_agreement":null},{"id":"W1990858385","doi":"10.1088/0004-637x/786/2/100","title":"MULTIWAVELENGTH OBSERVATIONS OF THE CANDIDATE DISINTEGRATING SUB-MERCURY KIC 12557548B, ,","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planet; Transit (satellite); Photometry (optics); Kepler; Spitzer Space Telescope; Telescope; Angular resolution (graph drawing); RADIUS","score_opus":0.013222718741738762,"score_gpt":0.2199296237910963,"score_spread":0.20670690504935751,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990858385","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975381,0.00010137243,0.00016950027,0.00002391038,0.0000040990813,0.000006289253,0.00032683718,0.00003686894,0.0017931734],"genre_scores_gemma":[0.9975345,0.0000351071,0.0008407827,0.000033473843,0.000004644532,0.000007013241,0.0009389351,0.0000062147974,0.0005992931],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999386,0.0000016866503,0.0000023860057,0.000022352022,0.000018687588,0.000016257642],"domain_scores_gemma":[0.9998801,0.0000047453764,0.000039293143,0.000010735982,0.000015614623,0.000049464325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000053702628,0.00022054494,0.00017642994,0.00089055125,0.00050023216,0.00023139523,0.00034989978,0.0003234701,0.0011512262],"category_scores_gemma":[0.0001309028,0.00015709677,0.00012537744,0.00039069884,0.00014983797,0.00013552776,0.0004412054,0.00023469079,0.00029613747],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004308912,0.00017265012,0.46640557,0.00011578951,0.00015577869,0.001138179,0.00061677094,0.0006724286,0.4840503,0.0003466603,0.002818733,0.043076288],"study_design_scores_gemma":[0.000015177421,0.00006287225,0.9897273,0.000007627117,0.000029096507,0.00040076723,0.000107051565,0.0008707838,0.006627244,0.000052791736,0.0020904543,0.000008880351],"about_ca_topic_score_codex":0.010182957,"about_ca_topic_score_gemma":0.045223285,"teacher_disagreement_score":0.010182957,"about_ca_system_score_codex":0.00039722578,"about_ca_system_score_gemma":0.00012705819,"threshold_uncertainty_score":0.02024734},"labels":[],"label_agreement":null},{"id":"W1990871593","doi":"10.1088/0004-637x/749/2/172","title":"PLANETESIMAL DYNAMICS IN INCLINED BINARY SYSTEMS: THE ROLE OF GAS-DISK GRAVITY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Physics; Eccentricity (behavior); Orbital plane; Drag; Orbit (dynamics); Astrophysics; Protoplanetary disk; Circular orbit; Planet; Dynamical friction; Giant planet; Planetary system; Astronomy; Mechanics","score_opus":0.00537036234602002,"score_gpt":0.20469952069174788,"score_spread":0.19932915834572787,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990871593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99535143,0.00048719012,0.0018683743,0.00010887742,0.000009173659,0.000008494424,0.000045274464,0.000022872366,0.00209832],"genre_scores_gemma":[0.99929667,0.00015133471,0.0003751692,0.000009276893,0.0000060574534,0.0000034418122,0.000022774464,0.00000567572,0.00012952505],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992526,0.000013750498,0.0000048910197,0.000016217444,0.00001179286,0.00002802553],"domain_scores_gemma":[0.99947864,0.00011190638,0.00024667667,0.000026255377,0.000032161795,0.0001044161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017661559,0.00040385057,0.0005214414,0.00052001665,0.0006390876,0.0008641741,0.00042651573,0.0004243845,0.00067677937],"category_scores_gemma":[0.0012751987,0.00017808459,0.0002828581,0.00049930415,0.0006611244,0.000772278,0.0010053847,0.00038335993,0.0001047993],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061802944,0.0003155661,0.2726892,0.0003050011,0.00027379574,0.0029922724,0.001500219,0.58706164,0.07996829,0.035629682,0.0009860459,0.017660303],"study_design_scores_gemma":[0.000062516105,0.00012852049,0.062752165,0.00001830337,0.00005626823,0.00027886542,0.00032805683,0.926679,0.0039729155,0.005047367,0.00063004176,0.000045972116],"about_ca_topic_score_codex":0.00596433,"about_ca_topic_score_gemma":0.0029867312,"teacher_disagreement_score":0.00596433,"about_ca_system_score_codex":0.0005599612,"about_ca_system_score_gemma":0.0002873665,"threshold_uncertainty_score":0.011859238},"labels":[],"label_agreement":null},{"id":"W1990940722","doi":"10.1088/0004-637x/732/2/97","title":"MAGNETIC FIELD STRUCTURE AROUND LOW-MASS CLASS 0 PROTOSTARS: B335, L1527, AND IC348-SMM2","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Magnetic field; Polarization (electrochemistry); Magnetic energy; Core (optical fiber); Magnetic structure; Pinch; Rotation (mathematics); Field (mathematics); Symmetry (geometry)","score_opus":0.00921594757176113,"score_gpt":0.21364352964956684,"score_spread":0.2044275820778057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1990940722","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996191,0.00001998035,0.000053457698,0.000003885662,3.986438e-7,0.0000010236549,0.000053600532,0.0000069130233,0.00024170635],"genre_scores_gemma":[0.9995559,0.000012511622,0.00011564161,0.0000042849524,0.0000017972691,0.000001223627,0.0002520746,0.0000024165327,0.000054133543],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995446,0.000003031326,0.0000021230026,0.000012706858,0.000012901843,0.000014776273],"domain_scores_gemma":[0.9998179,0.000014808067,0.00007047388,0.00001106397,0.000029834171,0.000055963086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007280815,0.00018872708,0.00017482067,0.0006684778,0.00024093835,0.00024849246,0.00025449853,0.00013126478,0.000565626],"category_scores_gemma":[0.00022156948,0.00010909855,0.00009301794,0.00038655745,0.00018675762,0.000107911175,0.00029696248,0.00015171603,0.0001494919],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037532745,0.000053048992,0.8624543,0.000032816584,0.000057723457,0.00039375038,0.00040140175,0.00091300305,0.12684472,0.00022085331,0.00032981983,0.007923334],"study_design_scores_gemma":[0.0000120348695,0.000030496069,0.99649787,0.0000026884481,0.000011180703,0.00008507643,0.000087200104,0.0009937128,0.0020157874,0.000037276015,0.000223022,0.000003642969],"about_ca_topic_score_codex":0.00782829,"about_ca_topic_score_gemma":0.012461982,"teacher_disagreement_score":0.00782829,"about_ca_system_score_codex":0.00033123852,"about_ca_system_score_gemma":0.000096955606,"threshold_uncertainty_score":0.015565455},"labels":[],"label_agreement":null},{"id":"W1991075961","doi":"10.1088/0004-637x/705/1/758","title":"PAndAS’ CUBS: DISCOVERY OF TWO NEW DWARF GALAXIES IN THE SURROUNDINGS OF THE ANDROMEDA AND TRIANGULUM GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Queen's University; University of Toronto; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Andromeda; Milky Way; Dwarf spheroidal galaxy; Local Group; Andromeda Galaxy; Dwarf galaxy; Galaxy","score_opus":0.009167373653624128,"score_gpt":0.2293094892159033,"score_spread":0.22014211556227917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991075961","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944007,0.0005460775,0.00031292453,0.000060609927,0.000013254842,0.0000074276663,0.00014570159,0.000035405417,0.004477938],"genre_scores_gemma":[0.99753785,0.00018947675,0.0009997888,0.000038965907,0.000011870813,0.000005915343,0.00035816393,0.000008970983,0.0008490572],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998568,0.000014600637,0.0000046271584,0.000054408614,0.000026667356,0.000042822085],"domain_scores_gemma":[0.9997631,0.00002456013,0.00007199834,0.00003809869,0.000026621738,0.0000756633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013936989,0.00019230395,0.00017025591,0.001015943,0.001052586,0.00093572895,0.00030268353,0.0002702402,0.0013595199],"category_scores_gemma":[0.0003245986,0.00018637266,0.00017402253,0.00074044464,0.00047061485,0.00028197438,0.0008889908,0.00026451715,0.00032105128],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029599285,0.000048597296,0.89557767,0.00010220757,0.00009096062,0.0037021348,0.0031417736,0.0001628547,0.03689463,0.0033889615,0.0016736937,0.05492062],"study_design_scores_gemma":[0.000010373694,0.00007969546,0.9551654,0.000023577644,0.000038392172,0.007730533,0.0018644144,0.00031608605,0.0037145892,0.0003774122,0.030657861,0.000021808877],"about_ca_topic_score_codex":0.004561868,"about_ca_topic_score_gemma":0.009751264,"teacher_disagreement_score":0.004561868,"about_ca_system_score_codex":0.00033602733,"about_ca_system_score_gemma":0.00018346136,"threshold_uncertainty_score":0.009070635},"labels":[],"label_agreement":null},{"id":"W1991301684","doi":"10.1086/341723","title":"On the Spectral Energy Dependence of Gamma‐Ray Burst Variability","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gamma-ray burst; Redshift; Physics; Astrophysics; Luminosity; Rest frame; Light curve; Absolute magnitude; Galaxy","score_opus":0.012064534108559934,"score_gpt":0.20837979211641722,"score_spread":0.1963152580078573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991301684","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99030346,0.0003553976,0.002456745,0.00007591268,0.000008662884,0.0000049016435,0.00032882072,0.00007313948,0.0063929125],"genre_scores_gemma":[0.9990085,0.00013361567,0.00025231665,0.000023990264,0.000015641966,0.0000027244237,0.0003081529,0.000027153152,0.00022808503],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998622,0.000029135737,0.000011276405,0.000034752527,0.000034494482,0.000028169636],"domain_scores_gemma":[0.9958811,0.0024113217,0.00075484277,0.00044991734,0.0003616815,0.00014111945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035301194,0.00016106178,0.00013375771,0.0011820153,0.00013025533,0.0007560646,0.00023286881,0.0003098501,0.001857043],"category_scores_gemma":[0.004941004,0.00015374817,0.00020835994,0.000842815,0.00031008947,0.0005833508,0.00035992565,0.00031912082,0.0005238678],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005225762,0.0000777164,0.87782335,0.000072190545,0.0001495117,0.0003913859,0.00029569387,0.005724806,0.07308672,0.0036262183,0.00060408935,0.03762573],"study_design_scores_gemma":[0.0000058416713,0.000034113495,0.98830324,0.000013697819,0.000026481208,0.00057403295,0.000053832915,0.006111479,0.0028786163,0.0014905315,0.0004947053,0.000013456625],"about_ca_topic_score_codex":0.00051687914,"about_ca_topic_score_gemma":0.0005132112,"teacher_disagreement_score":0.001857043,"about_ca_system_score_codex":0.00013513213,"about_ca_system_score_gemma":0.00006291613,"threshold_uncertainty_score":0.0062124133},"labels":[],"label_agreement":null},{"id":"W1991318814","doi":"10.1086/345980","title":"The Properties of Microjansky Radio Sources in the Hubble Deep Field–North, SSA 13, and SSA 22 Fields","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Redshift; Galaxy; Luminosity; Active galactic nucleus; Radio galaxy; Source counts; Hubble Deep Field; Population; COSMIC cancer database","score_opus":0.006308037187588919,"score_gpt":0.18365006935501813,"score_spread":0.17734203216742922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991318814","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952674,0.00003220217,0.000030852614,0.0000053912363,5.521188e-7,0.0000016917521,0.00017040699,0.0000030445588,0.00022913846],"genre_scores_gemma":[0.9992017,0.000038400543,0.000076067896,0.0000072155162,0.0000052857604,0.000003894514,0.0004971582,0.0000020153611,0.00016833191],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998971,0.0000077583945,0.00000815505,0.000031281004,0.000022565615,0.000033242362],"domain_scores_gemma":[0.9987948,0.0001420207,0.00054675876,0.00008982094,0.00012151278,0.00030498853],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019578704,0.00019542969,0.00019216446,0.0013648506,0.00028236554,0.0004085312,0.00019743222,0.00013456238,0.0009696032],"category_scores_gemma":[0.00064939796,0.00014526836,0.00013998683,0.00074940897,0.00024224022,0.00023738008,0.0003531782,0.00014403774,0.00018855836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000053996773,0.000018195162,0.9920832,0.000007061253,0.000024266035,0.00005137154,0.00022551802,0.000099055236,0.004256065,0.000045348414,0.00008967767,0.0030463205],"study_design_scores_gemma":[9.5278403e-7,0.0000056051867,0.9997662,8.134002e-7,0.0000030724057,0.000022672146,0.000027972077,0.00004115835,0.00007225534,0.0000062807158,0.00005214248,8.717743e-7],"about_ca_topic_score_codex":0.013776299,"about_ca_topic_score_gemma":0.030614432,"teacher_disagreement_score":0.013776299,"about_ca_system_score_codex":0.00028259124,"about_ca_system_score_gemma":0.00013340195,"threshold_uncertainty_score":0.027392209},"labels":[],"label_agreement":null},{"id":"W1991337674","doi":"10.1086/378689","title":"The MACHO Project Large Magellanic Cloud Variable Star Inventory. XI. Frequency Analysis of the Fundamental‐Mode RR Lyrae Stars","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"RR Lyrae variable; Physics; Astrophysics; Stars; Variable star; Large Magellanic Cloud; Overtone; Cepheid variable; Amplitude; Astronomy; Light curve; Instability strip; Stellar pulsation; Brightness; Spectral line; Globular cluster; Optics","score_opus":0.01158837384848613,"score_gpt":0.2412775441668687,"score_spread":0.22968917031838257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991337674","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04225649,0.0033223925,0.0020788037,0.0005293677,0.0002064806,0.00016917817,0.92144513,0.0013292694,0.028662853],"genre_scores_gemma":[0.07255025,0.0019719796,0.011729646,0.00012462337,0.00026966594,0.00036851972,0.89788383,0.00034666233,0.014754796],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996025,0.000027049648,0.00007008681,0.000039334114,0.00020651275,0.00005457534],"domain_scores_gemma":[0.9975472,0.00019961396,0.000737382,0.00020986106,0.00096355064,0.00034235686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006924133,0.00063232816,0.000550567,0.008396453,0.000396541,0.0009859129,0.0008665667,0.00023163715,0.010636854],"category_scores_gemma":[0.0022170383,0.00030773837,0.00032952038,0.0073047797,0.00013898437,0.00095601333,0.0016281821,0.00046224432,0.007222048],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083460944,0.00016382046,0.2136858,0.0009980283,0.00013476043,0.00014038228,0.0002940837,0.0006529484,0.0031141725,0.0047815535,0.54456973,0.23063019],"study_design_scores_gemma":[0.00008282024,0.00010643461,0.53473186,0.00020970382,0.00007663559,0.00025996938,0.00015994132,0.000778683,0.0017820611,0.0016100717,0.46017197,0.000029724462],"about_ca_topic_score_codex":0.01720797,"about_ca_topic_score_gemma":0.013601726,"teacher_disagreement_score":0.01720797,"about_ca_system_score_codex":0.00056064076,"about_ca_system_score_gemma":0.0011199756,"threshold_uncertainty_score":0.035583854},"labels":[],"label_agreement":null},{"id":"W1991391334","doi":"10.1088/0004-637x/745/1/95","title":"<i>HERSCHEL</i>FAR-INFRARED AND SUBMILLIMETER PHOTOMETRY FOR THE KINGFISH SAMPLE OF NEARBY GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":275,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Photometry (optics); Galaxy; Astronomy; Millimeter; Luminous infrared galaxy; Infrared; Far infrared; Black-body radiation; Cosmic dust; Radiation; Stars","score_opus":0.012416362873556495,"score_gpt":0.22682848160818408,"score_spread":0.2144121187346276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991391334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9147958,0.0007762071,0.0019866503,0.00023837495,0.000049122915,0.000099380464,0.06536458,0.0005138627,0.016176073],"genre_scores_gemma":[0.8886162,0.00035807813,0.005477245,0.00016729762,0.000056884168,0.00009144887,0.09571251,0.00018072047,0.009339642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995116,0.00002842599,0.000055809043,0.0001293734,0.00018579894,0.00008906361],"domain_scores_gemma":[0.9971776,0.00014701138,0.00096748373,0.00085783325,0.0004714456,0.0003785658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063232036,0.00027796737,0.00040760246,0.004281844,0.00039697066,0.0006246277,0.00061208685,0.0002449674,0.009685969],"category_scores_gemma":[0.0012948366,0.00026235537,0.0005124725,0.0019311575,0.00025630195,0.0007709266,0.0013072304,0.0003846166,0.005228658],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001674959,0.000032564494,0.9451147,0.00013280963,0.00014038479,0.00016882956,0.00040173533,0.000728424,0.015870752,0.000615517,0.0142287435,0.02239805],"study_design_scores_gemma":[0.0000049497135,0.000014239937,0.9912202,0.0000070212545,0.000010453032,0.00008337458,0.00006993799,0.00013953188,0.00059866754,0.00006786934,0.007775958,0.000007772939],"about_ca_topic_score_codex":0.029886255,"about_ca_topic_score_gemma":0.06515053,"teacher_disagreement_score":0.029886255,"about_ca_system_score_codex":0.0007571385,"about_ca_system_score_gemma":0.00054039626,"threshold_uncertainty_score":0.05942458},"labels":[],"label_agreement":null},{"id":"W1991484299","doi":"10.1088/0004-637x/721/1/738","title":"THE DUAL ORIGIN OF STELLAR HALOS. II. CHEMICAL ABUNDANCES AS TRACERS OF FORMATION HISTORY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Milky Way; Stars; Galactic halo; Galaxy; Metallicity; Halo; Galaxy formation and evolution; Star formation","score_opus":0.011611719416861366,"score_gpt":0.25757254811243857,"score_spread":0.2459608286955772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991484299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968665,0.00009147794,0.0020766049,0.00005051256,0.0000025845625,0.0000057507013,0.00007545948,0.00002788962,0.00080304296],"genre_scores_gemma":[0.9986809,0.000047595317,0.0009867733,0.000010251692,0.0000021642818,0.000004170462,0.00006269732,0.000010030499,0.00019544046],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999206,0.00003134798,0.0000038618423,0.000015592192,0.00001343275,0.000015177177],"domain_scores_gemma":[0.99952555,0.00013893534,0.00013701648,0.000061822575,0.000042570384,0.000094139876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040185935,0.00023490726,0.00017972254,0.0003008222,0.00021151153,0.00051376893,0.00051075546,0.00043628094,0.0004834346],"category_scores_gemma":[0.0017826138,0.00033139045,0.00031823126,0.00029297062,0.00063154945,0.0005358513,0.0007512151,0.0002446136,0.00011624788],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003442718,0.000078204284,0.3168489,0.00009445317,0.00018908993,0.00029688928,0.00041826954,0.6355915,0.023819603,0.01479054,0.00039778298,0.0071304245],"study_design_scores_gemma":[0.00010263888,0.00009082155,0.06045749,0.000010941486,0.000033254408,0.00010204031,0.0001223306,0.93062633,0.0032771165,0.0041713477,0.0009846583,0.000020983614],"about_ca_topic_score_codex":0.0071998215,"about_ca_topic_score_gemma":0.006072317,"teacher_disagreement_score":0.0071998215,"about_ca_system_score_codex":0.0006129146,"about_ca_system_score_gemma":0.00031965063,"threshold_uncertainty_score":0.014315844},"labels":[],"label_agreement":null},{"id":"W1991518800","doi":"10.1086/309507","title":"<i>EUVE</i>Observations of Hercules X‐1 during a Short High‐State Turn‐on","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Extreme ultraviolet lithography; Extreme ultraviolet; Accretion (finance); RADIUS; Black-body radiation; Neutron star; Bremsstrahlung","score_opus":0.014302154592048682,"score_gpt":0.22182195998584958,"score_spread":0.2075198053938009,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991518800","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.991884,0.0002415523,0.00021143947,0.00012130594,0.000018861432,0.000013849695,0.0012724992,0.000101143145,0.0061353296],"genre_scores_gemma":[0.9925966,0.00014694646,0.00074488303,0.00012393275,0.000041009473,0.000026061889,0.003755839,0.000041964053,0.0025227645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991596,0.0000074404115,0.0000034082816,0.00001876886,0.00002603565,0.000028405233],"domain_scores_gemma":[0.99978775,0.00002755787,0.00006009871,0.000030653675,0.00004353642,0.000050502364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018323079,0.00026029907,0.00026749072,0.0010989341,0.0006559435,0.0005302775,0.00027676809,0.00037615994,0.0012691794],"category_scores_gemma":[0.0002864264,0.00016341297,0.00017813775,0.0005183613,0.00015008636,0.00022065264,0.0007471421,0.00044697957,0.00025782862],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020372262,0.00045472226,0.67083097,0.0002410457,0.0004081898,0.0043205083,0.0017263886,0.0025088333,0.21743348,0.0010746474,0.018234143,0.080729865],"study_design_scores_gemma":[0.00001253765,0.000084631196,0.9919315,0.000015206958,0.000016116095,0.00043976257,0.000093957526,0.00030110165,0.0023508251,0.00006522862,0.0046778545,0.000011165774],"about_ca_topic_score_codex":0.0049500125,"about_ca_topic_score_gemma":0.015776036,"teacher_disagreement_score":0.0049500125,"about_ca_system_score_codex":0.0003684521,"about_ca_system_score_gemma":0.0001233334,"threshold_uncertainty_score":0.009842396},"labels":[],"label_agreement":null},{"id":"W1991620768","doi":"10.1086/381217","title":"The Canada‐UK Deep Submillimeter Survey. VII. Optical and Near‐Infrared Identifications for the 14 Hour Field","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"","keywords":"Redshift; Astrophysics; Physics; Population; Infrared; Flux (metallurgy); Redshift survey; Limit (mathematics); Astronomy; Galaxy; Hubble Deep Field; Observational cosmology; Demography; Chemistry","score_opus":0.010378108072557018,"score_gpt":0.22016002232809498,"score_spread":0.20978191425553797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991620768","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.48332155,0.004443781,0.0027889234,0.0022946573,0.0003058067,0.00032747185,0.43414795,0.00049568777,0.07187414],"genre_scores_gemma":[0.72157556,0.0023603959,0.005541461,0.0005754555,0.00008238111,0.00023481763,0.210106,0.0000870235,0.05943692],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968636,0.0000090054,0.0000131843535,0.000026192625,0.0001391744,0.00012606126],"domain_scores_gemma":[0.99859494,0.000043251133,0.0002431057,0.000073062925,0.0007455056,0.00030008095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025608967,0.0002979167,0.00020489257,0.0040195794,0.0009881402,0.00061032875,0.00055644993,0.00022886187,0.007868677],"category_scores_gemma":[0.0010845321,0.00017037721,0.00019034652,0.004005428,0.00022665274,0.0002731919,0.00068828627,0.00026888837,0.0016736973],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020561568,0.000035147452,0.6469473,0.00018878451,0.000064673004,0.0001900461,0.00075965247,0.0006511572,0.0019446918,0.0033522556,0.24782668,0.097834],"study_design_scores_gemma":[0.000012728401,0.000008068049,0.91962576,0.00003352844,0.000013002204,0.000046365585,0.00024014234,0.00026598424,0.00034772168,0.00013625837,0.07926094,0.000009395024],"about_ca_topic_score_codex":0.967346,"about_ca_topic_score_gemma":0.9830875,"teacher_disagreement_score":0.967346,"about_ca_system_score_codex":0.009148665,"about_ca_system_score_gemma":0.008421012,"threshold_uncertainty_score":0.06637859},"labels":[],"label_agreement":null},{"id":"W1991635028","doi":"10.1086/591633","title":"Development of Flux Imbalances in Solar Activity Nests and the Evolution of Filament Channels","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Protein filament; Physics; Flux (metallurgy); Magnetic flux; Sunspot; Astrophysics; Line (geometry); Magnetic field; Geometry; Biology; Chemistry","score_opus":0.008047847836808853,"score_gpt":0.21536593291512227,"score_spread":0.20731808507831342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991635028","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990459,0.000024720426,0.00035028407,0.000008423144,7.9162794e-7,0.0000015450843,0.000014051064,0.000007969049,0.00054625695],"genre_scores_gemma":[0.9997209,0.0000125998595,0.00014473121,0.0000019517192,0.0000014588442,0.0000012013168,0.000025152336,0.000002527703,0.00008958823],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999925,0.000009339119,0.000004157474,0.000018446985,0.000015493779,0.00002757961],"domain_scores_gemma":[0.9996344,0.000049429404,0.00017614993,0.000026487212,0.000040925417,0.00007267807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000103161525,0.00008232121,0.00014659726,0.0005771528,0.00034402785,0.0006269618,0.00016899015,0.0002571871,0.0006878033],"category_scores_gemma":[0.0007557249,0.00014035091,0.00012275638,0.00024328458,0.00038538134,0.00047249935,0.00043064516,0.00016718484,0.00010526482],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005651971,0.00007686434,0.7209942,0.0000380701,0.000056319575,0.0016386602,0.0017149529,0.006952776,0.24199039,0.0040102643,0.00042848557,0.021533828],"study_design_scores_gemma":[0.000014994911,0.0000933336,0.9783407,0.000008180903,0.000019308036,0.0011249312,0.0006313892,0.008216416,0.009064806,0.0013439301,0.0011247038,0.000017249049],"about_ca_topic_score_codex":0.0010537786,"about_ca_topic_score_gemma":0.0009053085,"teacher_disagreement_score":0.0010537786,"about_ca_system_score_codex":0.00031213782,"about_ca_system_score_gemma":0.00008669238,"threshold_uncertainty_score":0.002300918},"labels":[],"label_agreement":null},{"id":"W1991640199","doi":"10.1088/0004-637x/699/2/l165","title":"FAR-INFRARED DETECTION OF NEUTRAL ATOMIC OXYGEN TOWARD THE HORSEHEAD NEBULA","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Radiative transfer; Astrophysics; Nebula; Collisional excitation; Infrared; Photodissociation; Line (geometry); Wavelength; Luminosity; Spectral energy distribution; Emission spectrum; Spectral line; Atomic physics; Spitzer Space Telescope; Ion; Astronomy; Galaxy; Telescope; Optics; Ionization; Stars; Chemistry","score_opus":0.01097274961402526,"score_gpt":0.23477056921712985,"score_spread":0.2237978196031046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991640199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979032,0.00012829922,0.0004510111,0.000018459563,0.000004346229,0.0000038090297,0.00004688085,0.000016147986,0.0014278824],"genre_scores_gemma":[0.99821293,0.00004882106,0.00083743286,0.000023852555,0.000008550067,0.0000023034916,0.00011318634,0.000003750278,0.0007490727],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994373,0.0000018643262,0.000001042377,0.00002230163,0.000018168086,0.00001289623],"domain_scores_gemma":[0.99990404,0.0000107209735,0.000027551245,0.000010177875,0.000017368533,0.000030166459],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000640393,0.00012679385,0.00007691032,0.00028088392,0.00026862265,0.0002390116,0.00037595344,0.00035295155,0.001196591],"category_scores_gemma":[0.00015323695,0.00012190402,0.00007438799,0.00011402046,0.00029870422,0.00022581624,0.00030681674,0.00016209805,0.0001896722],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021742305,0.00007047923,0.1434629,0.00009105203,0.00003329165,0.0010374835,0.0004833107,0.00012989956,0.838323,0.00047097102,0.0004460899,0.015234094],"study_design_scores_gemma":[0.00002611679,0.0005726717,0.8850893,0.000022659024,0.00003704034,0.002409899,0.00020751855,0.0015256201,0.1032322,0.00038555902,0.0064753024,0.000016080745],"about_ca_topic_score_codex":0.0015675895,"about_ca_topic_score_gemma":0.004417931,"teacher_disagreement_score":0.0015675895,"about_ca_system_score_codex":0.00013548952,"about_ca_system_score_gemma":0.00007228729,"threshold_uncertainty_score":0.0040029883},"labels":[],"label_agreement":null},{"id":"W1991787827","doi":"10.1086/519945","title":"Multi‐ionic Kinematical Study of the H<scp>ii</scp>Region Sharpless 2‐158","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Line width; Line (geometry); Molecular cloud; Spectral line; Ion; Radial velocity; Stars; Field (mathematics); Atomic physics; Geometry; Astronomy; Optics","score_opus":0.019745759433639612,"score_gpt":0.2668410968382747,"score_spread":0.24709533740463513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991787827","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99797815,0.000041966043,0.00016790145,0.000013666424,0.0000015405211,0.000003974464,0.00016118525,0.000017152182,0.0016145048],"genre_scores_gemma":[0.9990256,0.000027856753,0.00018976278,0.000007379989,0.0000041174894,0.000002560438,0.00043269023,0.000010637293,0.0002992648],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999236,0.000004090913,0.0000038289877,0.000026716205,0.000020728508,0.000021073778],"domain_scores_gemma":[0.999876,0.00001788297,0.000040905295,0.0000080414675,0.000022449616,0.000034797977],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011233721,0.00021210972,0.00018366546,0.0012262891,0.0003817824,0.0006086105,0.00028284837,0.00015680837,0.0012512268],"category_scores_gemma":[0.00022891162,0.00019941154,0.00019460334,0.0006214189,0.00028995704,0.00031071357,0.00054584263,0.00013881603,0.00024078586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035310673,0.00007961965,0.8408429,0.00005423481,0.00011418753,0.0013557617,0.0006193553,0.0016751403,0.14112848,0.00079411257,0.00047069628,0.012512401],"study_design_scores_gemma":[0.000017805822,0.0000702849,0.990137,0.0000059839726,0.000021704025,0.0003512091,0.00028483066,0.0033158108,0.004374102,0.00015598504,0.0012564849,0.00000882399],"about_ca_topic_score_codex":0.00767326,"about_ca_topic_score_gemma":0.006486638,"teacher_disagreement_score":0.00767326,"about_ca_system_score_codex":0.0003400401,"about_ca_system_score_gemma":0.0002021437,"threshold_uncertainty_score":0.01525718},"labels":[],"label_agreement":null},{"id":"W1991913308","doi":"10.1088/0004-637x/757/1/12","title":"A SEARCH FOR NEW CANDIDATE SUPER-CHANDRASEKHAR-MASS TYPE Ia SUPERNOVAE IN THE NEARBY SUPERNOVA FACTORY DATA SET","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Supernova; Chandrasekhar limit; White dwarf; Physics; Astrophysics; Light curve; Common envelope; Ejecta; Population; Photometry (optics); Astronomy; Stars","score_opus":0.0562909923953318,"score_gpt":0.31138308166508405,"score_spread":0.25509208926975224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991913308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99633527,0.000068061396,0.00017664074,0.000017098,0.000003618561,0.000010309717,0.0028132058,0.000028034661,0.00054780615],"genre_scores_gemma":[0.96288466,0.000058247933,0.00081232464,0.000039732095,0.000012194767,0.000024440818,0.03578267,0.000011191145,0.00037450448],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996519,0.000024244739,0.000038720525,0.00009687275,0.00010675227,0.00008149898],"domain_scores_gemma":[0.99835014,0.00016628117,0.0004913835,0.0002705486,0.00015041161,0.00057124475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051564176,0.00032851065,0.0003607248,0.002627262,0.0005555337,0.00073152705,0.0005296584,0.00030942677,0.0016933405],"category_scores_gemma":[0.00086443766,0.00015792671,0.0004739817,0.001629266,0.00016421363,0.00019241858,0.00054939016,0.00020157378,0.0005742692],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027236142,0.00011053747,0.9803919,0.00002395173,0.00009038565,0.00052293914,0.0001151039,0.00043896263,0.009599606,0.00017092629,0.0010128694,0.007250369],"study_design_scores_gemma":[0.000019464687,0.000039499966,0.99477994,0.000005960692,0.000024307737,0.00057017035,0.00012375512,0.0009265185,0.0012436343,0.000043962937,0.0022156376,0.0000070607307],"about_ca_topic_score_codex":0.0072457143,"about_ca_topic_score_gemma":0.015615257,"teacher_disagreement_score":0.0072457143,"about_ca_system_score_codex":0.0002909481,"about_ca_system_score_gemma":0.00046513946,"threshold_uncertainty_score":0.014407098},"labels":[],"label_agreement":null},{"id":"W1991941183","doi":"10.1086/430342","title":"The ACS Virgo Cluster Survey. VII. Resolving the Connection between Globular Clusters and Ultracompact Dwarf Galaxies","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":288,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Dwarf galaxy; Astronomy; Virgo Cluster; Star cluster; Galaxy; Elliptical galaxy; Galaxy cluster","score_opus":0.010731592094687843,"score_gpt":0.22916704987119618,"score_spread":0.21843545777650833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1991941183","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.02005958,0.007948902,0.0014109708,0.0063472465,0.002480481,0.0005712873,0.93744797,0.0026053158,0.021128261],"genre_scores_gemma":[0.03965155,0.0055139633,0.008913654,0.0026279483,0.0015797951,0.00070818356,0.92483777,0.0005636198,0.015603467],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9984143,0.00015967655,0.00017279567,0.00015614837,0.00079246063,0.00030461975],"domain_scores_gemma":[0.9909039,0.0007335171,0.001333668,0.000895715,0.003968702,0.0021645762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0031308685,0.002779303,0.0023654297,0.011770131,0.0015920883,0.003555481,0.0032345515,0.0020897565,0.0110422205],"category_scores_gemma":[0.006686691,0.0017107689,0.0011981119,0.013236828,0.0007376841,0.0016219475,0.003430473,0.002714468,0.0103208395],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020356402,0.00014648428,0.026366413,0.00048947724,0.0001948323,0.00013955995,0.00007675011,0.00047780076,0.0007655599,0.0006953996,0.94196796,0.028476138],"study_design_scores_gemma":[0.00067459414,0.00014895208,0.51030064,0.0006689838,0.00067773316,0.00023524405,0.00045744897,0.000989527,0.0026780518,0.0025251522,0.48048016,0.00016344027],"about_ca_topic_score_codex":0.16958626,"about_ca_topic_score_gemma":0.18229094,"teacher_disagreement_score":0.16958626,"about_ca_system_score_codex":0.0033722972,"about_ca_system_score_gemma":0.0045049614,"threshold_uncertainty_score":0.33719826},"labels":[],"label_agreement":null},{"id":"W1992016754","doi":"10.1088/0004-637x/703/1/240","title":"FOLLOW-UP OBSERVATIONS OF THE SECOND AND THIRD KNOWN PULSATING HOT DQ WHITE DWARFS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Astrophysics; Light curve; Amplitude; Oscillation (cell signaling); Luminosity; Sign (mathematics); Pulse (music); Series (stratigraphy); Period (music); Stars; Optics","score_opus":0.01704343121793102,"score_gpt":0.22500771967004735,"score_spread":0.2079642884521163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992016754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976706,0.00009148427,0.0003512773,0.000021822392,0.000008789121,0.0000090166095,0.00023961895,0.000024703639,0.0015827374],"genre_scores_gemma":[0.99626285,0.00006540657,0.00073118124,0.00004768369,0.0000217684,0.000010959427,0.001160249,0.000010396304,0.0016894796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998667,0.000006438208,0.000005006828,0.000041212646,0.000045063174,0.00003555335],"domain_scores_gemma":[0.9995478,0.000033287964,0.000101088146,0.00004949752,0.00008297224,0.00018539802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024961494,0.00018049845,0.0003159886,0.0010023495,0.00056048797,0.00045504447,0.00024237492,0.00031817332,0.0010557737],"category_scores_gemma":[0.00040967506,0.0001244733,0.00021186395,0.000525547,0.00021010452,0.00026447175,0.0007852142,0.00057379296,0.00044214807],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041448287,0.00035935405,0.7537358,0.000103905855,0.0000833727,0.0021982999,0.0025734196,0.00030471061,0.2061158,0.00067926256,0.0012664911,0.032165106],"study_design_scores_gemma":[0.000009924486,0.00018374849,0.9853554,0.0000061838355,0.000021770296,0.0009210919,0.00028866014,0.00031475004,0.0075166323,0.00013114116,0.0052364925,0.00001422919],"about_ca_topic_score_codex":0.0019434792,"about_ca_topic_score_gemma":0.0045552813,"teacher_disagreement_score":0.0019434792,"about_ca_system_score_codex":0.00027436521,"about_ca_system_score_gemma":0.00012288685,"threshold_uncertainty_score":0.0038642883},"labels":[],"label_agreement":null},{"id":"W1992045523","doi":"10.1086/500496","title":"Outflows and Jets from Collapsing Magnetized Cloud Cores","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":246,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Protostar; Outflow; Magnetic field; Magnetohydrodynamics; Angular momentum; Toroid; Herbig–Haro object; Jet (fluid); Star formation; Molecular cloud","score_opus":0.00726661765653964,"score_gpt":0.2169166884120533,"score_spread":0.20965007075551367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992045523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959757,0.000053936412,0.0020838452,0.000034061675,0.0000122890815,0.000020249177,0.000112971444,0.00004829432,0.0016586046],"genre_scores_gemma":[0.99747354,0.000051276973,0.0015480354,0.000023579365,0.0000059052168,0.000016654769,0.0002307753,0.000018523087,0.00063166046],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999312,0.000011829166,0.0000038590847,0.000010723126,0.000015409056,0.000026978923],"domain_scores_gemma":[0.99980885,0.00004955873,0.000046278874,0.00001016138,0.00001569196,0.00006950085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012627261,0.0003492664,0.00033680617,0.00028218093,0.00047125813,0.00073027436,0.0005738873,0.0005399081,0.0011435187],"category_scores_gemma":[0.00056036614,0.00023094098,0.0004413221,0.00026354796,0.0005090519,0.000281357,0.000501357,0.00030076256,0.00008762224],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031955005,0.00016419406,0.029190918,0.00006614879,0.00010894199,0.0008707662,0.00016621257,0.95198965,0.012242997,0.0019225363,0.00034819404,0.0026099766],"study_design_scores_gemma":[0.000144207,0.00011732245,0.016291771,0.000011786249,0.000020064503,0.000117925054,0.000107401385,0.9788302,0.002946405,0.00078173843,0.00061753904,0.000013702898],"about_ca_topic_score_codex":0.015307368,"about_ca_topic_score_gemma":0.008567317,"teacher_disagreement_score":0.015307368,"about_ca_system_score_codex":0.0007253423,"about_ca_system_score_gemma":0.000595878,"threshold_uncertainty_score":0.030436516},"labels":[],"label_agreement":null},{"id":"W1992202274","doi":"10.1088/0004-637x/795/1/54","title":"DELAYED STAR FORMATION IN ISOLATED DWARF GALAXIES:<i>HUBBLE SPACE TELESCOPE</i>STAR FORMATION HISTORY OF THE AQUARIUS DWARF IRREGULAR","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Star formation; Astronomy; Galaxy; Dwarf spheroidal galaxy; Stellar mass; Metallicity; Irregular galaxy; Advanced Camera for Surveys; Globular cluster; Lenticular galaxy","score_opus":0.00649714018990917,"score_gpt":0.18867368892530353,"score_spread":0.18217654873539435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992202274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990717,0.00007149253,0.00010207477,0.000011553408,0.0000016134663,0.0000019424886,0.0002241305,0.000010021848,0.00050530967],"genre_scores_gemma":[0.9993049,0.000026694404,0.00014576367,0.000007443023,0.0000028688814,0.0000013880946,0.00034593177,0.0000028410502,0.00016212367],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994075,0.0000062354,0.00000418064,0.000024808209,0.000009749366,0.000014285038],"domain_scores_gemma":[0.99946564,0.000052917345,0.00020328826,0.000063542735,0.00004522295,0.0001693888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017845735,0.00014049927,0.00015141658,0.00058447715,0.00023109141,0.00031590517,0.000222668,0.000109721295,0.0007616611],"category_scores_gemma":[0.00048036248,0.0000967896,0.00012984968,0.0004444975,0.00028998053,0.0002053943,0.00036059812,0.00020675852,0.00015500379],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020235057,0.000051867763,0.96499765,0.000023250204,0.00005064069,0.00024226372,0.0002777546,0.00079552183,0.02657527,0.00020885671,0.00016642174,0.006408144],"study_design_scores_gemma":[0.0000030475383,0.000034309538,0.9976447,0.0000021967035,0.000007973961,0.000098562676,0.00002973431,0.00036212098,0.0013855764,0.000054121214,0.000374149,0.0000034574193],"about_ca_topic_score_codex":0.011755957,"about_ca_topic_score_gemma":0.014914761,"teacher_disagreement_score":0.011755957,"about_ca_system_score_codex":0.0005047279,"about_ca_system_score_gemma":0.00014122082,"threshold_uncertainty_score":0.023375034},"labels":[],"label_agreement":null},{"id":"W1992250918","doi":"10.1086/308274","title":"The Evolution of AmFm Stars, Abundance Anomalies, and Turbulent Transport","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":270,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Compute Canada","funders":"","keywords":"Physics; Astrophysics; Stars; Convection zone; Turbulence; Radiative transfer; Abundance (ecology); Stellar evolution; Convection; Astronomy; Thermodynamics","score_opus":0.005299438975080316,"score_gpt":0.1956633713584645,"score_spread":0.1903639323833842,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992250918","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946024,0.00005003354,0.0036526616,0.00004944992,0.0000051273146,0.000004485989,0.00013067841,0.00006723669,0.0014379397],"genre_scores_gemma":[0.99840623,0.00002130332,0.0010522761,0.0000077110935,0.000002507198,0.0000043302816,0.00016143966,0.00001951475,0.00032468615],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99989426,0.000023334449,0.0000057664242,0.000023140763,0.000026361276,0.00002716878],"domain_scores_gemma":[0.9997328,0.00006051726,0.000062934174,0.00003036427,0.00005731107,0.000056099598],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032862122,0.0003570256,0.0002696678,0.00055163173,0.00048608135,0.0006849673,0.00047214952,0.0005940973,0.00047422622],"category_scores_gemma":[0.0012726076,0.00023105681,0.0006477377,0.00034488327,0.00036946315,0.00047906383,0.0003781637,0.00032476452,0.00018045318],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018662575,0.000047823392,0.17219478,0.000034056477,0.00008868743,0.00037665226,0.00017252835,0.7917131,0.014480326,0.014310697,0.0004099383,0.0059848214],"study_design_scores_gemma":[0.000020209693,0.000046759884,0.032022864,0.000006094705,0.00001391844,0.0001982087,0.000041662384,0.9623208,0.0020042085,0.0027050122,0.0006012244,0.00001897113],"about_ca_topic_score_codex":0.008359964,"about_ca_topic_score_gemma":0.0033139372,"teacher_disagreement_score":0.008359964,"about_ca_system_score_codex":0.0015672335,"about_ca_system_score_gemma":0.00028969868,"threshold_uncertainty_score":0.016622603},"labels":[],"label_agreement":null},{"id":"W1992287913","doi":"10.1088/0004-637x/798/1/7","title":"OVERVIEW OF THE SDSS-IV MaNGA SURVEY: MAPPING NEARBY GALAXIES AT APACHE POINT OBSERVATORY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1669,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Sky; Observatory; Context (archaeology); Stars; Luminosity; Redshift; Star formation; Extragalactic astronomy; Luminous infrared galaxy","score_opus":0.029203917852893488,"score_gpt":0.2285002531372384,"score_spread":0.19929633528434493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992287913","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17149657,0.06322026,0.033058457,0.006913103,0.0009215629,0.004133486,0.5709809,0.00965797,0.1396177],"genre_scores_gemma":[0.19595608,0.044786308,0.11800135,0.0029675076,0.0023376988,0.003228844,0.59643143,0.0019636,0.034327295],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99925977,0.00006974626,0.00005518509,0.000185699,0.00031849818,0.0001110793],"domain_scores_gemma":[0.99869066,0.000086587446,0.00019517973,0.00015333194,0.00050514174,0.00036912947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001458693,0.00074026856,0.00046895348,0.0059436522,0.000627641,0.0009894614,0.000913552,0.00030705085,0.0071069393],"category_scores_gemma":[0.0010824089,0.000511399,0.0003204687,0.0059435396,0.00022781164,0.0009957749,0.0012896133,0.00051026425,0.004393911],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002472938,0.00018698342,0.24439454,0.0017636461,0.00017938044,0.0001809435,0.0005608478,0.002114126,0.010026013,0.0036721241,0.41404074,0.32263327],"study_design_scores_gemma":[0.000028410579,0.00006252614,0.385689,0.0003198906,0.00004606635,0.0001676166,0.00021364543,0.0005894969,0.00066397915,0.0009718489,0.6112115,0.000036044657],"about_ca_topic_score_codex":0.06425503,"about_ca_topic_score_gemma":0.05599309,"teacher_disagreement_score":0.06425503,"about_ca_system_score_codex":0.0015976316,"about_ca_system_score_gemma":0.0024116659,"threshold_uncertainty_score":0.12776202},"labels":[],"label_agreement":null},{"id":"W1992385960","doi":"10.1086/324494","title":"Deep Submillimeter Imaging of Dust Structures in Centaurus A","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Centaurus A; Physics; Astrophysics; Surface brightness; Infrared; Spectral energy distribution; Brightness; Dust lane; Astronomy; RADIUS; Star formation; Submillimeter Array; Wavelength; Millimeter; Galaxy; Active galactic nucleus; Optics","score_opus":0.010118445372719125,"score_gpt":0.22300774032929674,"score_spread":0.2128892949565776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992385960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985429,0.00012214652,0.00016149055,0.000013596255,0.0000034021446,0.0000023940022,0.00016869036,0.000031197203,0.000954111],"genre_scores_gemma":[0.99921834,0.000043600103,0.00032477552,0.000014002491,0.0000064604105,0.000002764827,0.000167583,0.0000036171632,0.00021898172],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995327,0.0000028188879,0.0000027516612,0.000015741083,0.000010291415,0.000015214657],"domain_scores_gemma":[0.99977475,0.000027427595,0.000060025588,0.000021643633,0.000022654272,0.00009346809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008657078,0.00017152935,0.00017676705,0.0014037398,0.00030485122,0.00046138195,0.00023479306,0.0002150267,0.0007988384],"category_scores_gemma":[0.00022969826,0.00021318269,0.00017143827,0.00042512506,0.00018003161,0.0001753706,0.00055479526,0.00021665683,0.00022577318],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004678009,0.00011029909,0.37147495,0.000119803,0.0001388458,0.0013068016,0.00101814,0.001014014,0.59297013,0.00041201749,0.0007338004,0.030233383],"study_design_scores_gemma":[0.000003679259,0.000028355984,0.99708146,0.0000043972436,0.000010440948,0.00021491345,0.00009702218,0.00030155826,0.0018732495,0.000040866234,0.0003400264,0.0000039440624],"about_ca_topic_score_codex":0.002919219,"about_ca_topic_score_gemma":0.0049728327,"teacher_disagreement_score":0.002919219,"about_ca_system_score_codex":0.0002783665,"about_ca_system_score_gemma":0.000078332196,"threshold_uncertainty_score":0.0058044195},"labels":[],"label_agreement":null},{"id":"W1992400176","doi":"10.1088/0004-637x/758/1/11","title":"A BAYESIAN APPROACH TO LOCATING THE RED GIANT BRANCH TIP MAGNITUDE. II. DISTANCES TO THE SATELLITES OF M31","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":177,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Red-giant branch; Markov chain Monte Carlo; Magnitude (astronomy); Physics; Bayesian probability; Absolute magnitude; Posterior probability; Local Group; Algorithm; Astrophysics; Stars; Mathematics; Statistics; Milky Way; Globular cluster","score_opus":0.013240583388248734,"score_gpt":0.22750533679022253,"score_spread":0.2142647534019738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992400176","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.011493661,0.00028040275,0.9845233,0.00032603438,0.000021690887,0.00003701452,0.00019462722,0.00024183824,0.002881453],"genre_scores_gemma":[0.24173233,0.0007312474,0.75144935,0.00023236322,0.00013895171,0.00019258117,0.0007063053,0.00017828844,0.0046385555],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99929035,0.00020439479,0.00003776999,0.00015877272,0.00026048272,0.000048156668],"domain_scores_gemma":[0.99884284,0.0005306298,0.00017077179,0.00011884319,0.0002715936,0.00006532541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016551237,0.00043224255,0.00046508052,0.0022795745,0.00075590465,0.0016487531,0.0015081643,0.0009473762,0.0023219427],"category_scores_gemma":[0.006731841,0.0007232105,0.00060250395,0.0011397728,0.00081575685,0.0014602469,0.0014870777,0.0010432781,0.00072499126],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010773969,0.00007998849,0.011844545,0.00018583122,0.00014856858,0.0001852404,0.000452168,0.4146857,0.009653501,0.22689532,0.0051187724,0.33064267],"study_design_scores_gemma":[0.000024735251,0.000031160944,0.006019386,0.00006609498,0.000030854233,0.00022707318,0.000084973166,0.8164858,0.0028493828,0.16403507,0.01007722,0.00006821284],"about_ca_topic_score_codex":0.0085056,"about_ca_topic_score_gemma":0.011189537,"teacher_disagreement_score":0.0085056,"about_ca_system_score_codex":0.001483757,"about_ca_system_score_gemma":0.0016519042,"threshold_uncertainty_score":0.016912222},"labels":[],"label_agreement":null},{"id":"W1992561743","doi":"10.1086/427080","title":"Discovery of a Cool, Massive, and Metal-rich DAZ White Dwarf","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Surface gravity; Astrophysics; Physics; Effective temperature; Atmosphere (unit); Metal; Spectral line; Accretion (finance); Star (game theory); Stars; Astronomy; Chemistry; Thermodynamics","score_opus":0.008846052459533146,"score_gpt":0.2173313983786094,"score_spread":0.20848534591907625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992561743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99627966,0.0006620624,0.00086945953,0.00017537469,0.000024688212,0.000007418424,0.00022899845,0.00006233053,0.0016900398],"genre_scores_gemma":[0.9947843,0.00047085038,0.0023715221,0.0001209253,0.000047497047,0.000004999215,0.00071475125,0.00000894135,0.0014761321],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999409,0.0000025414824,0.000003236284,0.000020795436,0.000019125013,0.000013506268],"domain_scores_gemma":[0.99989974,0.0000064730584,0.000028535289,0.000012124838,0.000010246032,0.000042891523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001098881,0.0003053958,0.00023636897,0.0003709007,0.0004071376,0.00059126946,0.00032958508,0.00052244036,0.00033485112],"category_scores_gemma":[0.00018194593,0.00012282276,0.00014377043,0.00023648032,0.00039063592,0.00036745222,0.0006092745,0.0003461998,0.00026808894],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005947938,0.00008193526,0.17116995,0.00019077497,0.00007001319,0.010069875,0.00073375966,0.0006351281,0.7752757,0.006365185,0.0017212522,0.033091564],"study_design_scores_gemma":[0.000088161636,0.0012973067,0.5676965,0.00002929223,0.00018325254,0.03518117,0.0006479504,0.0036766438,0.28038168,0.005683275,0.10506337,0.00007147866],"about_ca_topic_score_codex":0.0010124312,"about_ca_topic_score_gemma":0.0014012114,"teacher_disagreement_score":0.0010124312,"about_ca_system_score_codex":0.00030105805,"about_ca_system_score_gemma":0.00015004171,"threshold_uncertainty_score":0.002184391},"labels":[],"label_agreement":null},{"id":"W1992575764","doi":"10.1086/318907","title":"Ultra–High-Density Molecular Core and Warped Nuclear Disk in the Deep Potential of Radio Lobe Galaxy NGC 3079","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Spiral galaxy; RADIUS; Galaxy rotation curve; Galaxy; Dust lane; Differential rotation; Telescope; Rotation (mathematics); Interferometry","score_opus":0.006137793124210194,"score_gpt":0.21044072260182037,"score_spread":0.20430292947761017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992575764","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992926,0.000085510044,0.00010329797,0.000012550698,0.0000012544133,9.605619e-7,0.00004852369,0.0000046308182,0.00045065957],"genre_scores_gemma":[0.9996729,0.00002439375,0.00011151686,0.0000047395956,0.0000014181558,0.000001101711,0.00010036542,0.0000013256499,0.00008222777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995613,0.000005250794,0.00000254156,0.000012131906,0.000010587087,0.000013385795],"domain_scores_gemma":[0.9998572,0.0000128399415,0.00003937304,0.00001735189,0.000016818334,0.00005642779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000093504306,0.0001562357,0.0001699808,0.0003441932,0.00032602306,0.0002942095,0.00021698118,0.00016144986,0.00063413964],"category_scores_gemma":[0.00019897016,0.00014388387,0.00010484158,0.00022653134,0.00026601233,0.00022022346,0.00041334212,0.00013358373,0.00024133816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037855422,0.00006452028,0.6899241,0.000049664744,0.000061764105,0.0017325452,0.00058155856,0.0015723831,0.29755253,0.001166047,0.00029822942,0.0066181617],"study_design_scores_gemma":[0.000021894431,0.00012199138,0.98783934,0.00001348028,0.000025550795,0.0009904592,0.00036012233,0.0024390207,0.005960229,0.00074790884,0.0014663119,0.000013711145],"about_ca_topic_score_codex":0.0026149636,"about_ca_topic_score_gemma":0.0049536703,"teacher_disagreement_score":0.0026149636,"about_ca_system_score_codex":0.00029203782,"about_ca_system_score_gemma":0.00010218344,"threshold_uncertainty_score":0.005199492},"labels":[],"label_agreement":null},{"id":"W1992775277","doi":"10.1088/0004-637x/698/2/1020","title":"MAPPING CRUSTAL HEATING WITH THE COOLING LIGHT CURVES OF QUASI-PERSISTENT TRANSIENTS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Neutron star; Thermal; Thermal conductivity; Thermal radiation; Cooling curve; Neutron; Crust; Thermal emission","score_opus":0.012305390903902326,"score_gpt":0.2812046407469561,"score_spread":0.2688992498430538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992775277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967483,0.000043388918,0.0025291042,0.00000806163,9.2553483e-7,0.0000035581163,0.00008908595,0.000071680945,0.00050579186],"genre_scores_gemma":[0.9986933,0.00002776049,0.0010570687,0.0000017440852,0.0000010832691,0.0000019154736,0.00012383044,0.000022554357,0.000070865906],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999943,0.000011254508,0.0000023881037,0.000017521807,0.000010020443,0.000015843256],"domain_scores_gemma":[0.9996227,0.000073430754,0.00012328479,0.00008266307,0.000034369532,0.00006356303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021809376,0.0002688858,0.00017734527,0.0006669155,0.0001796439,0.00049969985,0.00032354228,0.00025988944,0.0007466552],"category_scores_gemma":[0.0008768135,0.00027170687,0.00055970857,0.00062918745,0.0002562091,0.00027220364,0.00037869133,0.00030025345,0.00015631349],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009592517,0.00014566614,0.5556854,0.000118586664,0.00021446707,0.0005775356,0.00094678806,0.21304038,0.19276652,0.0031655806,0.0003902409,0.031989627],"study_design_scores_gemma":[0.000027738011,0.00010817832,0.65358734,0.00002253904,0.000052052143,0.0003146264,0.00017768088,0.32742333,0.015681576,0.0015008248,0.0010683294,0.00003579102],"about_ca_topic_score_codex":0.0043777763,"about_ca_topic_score_gemma":0.0029118834,"teacher_disagreement_score":0.0043777763,"about_ca_system_score_codex":0.00044635838,"about_ca_system_score_gemma":0.00015870748,"threshold_uncertainty_score":0.008704603},"labels":[],"label_agreement":null},{"id":"W1992865401","doi":"10.1086/507454","title":"Comparison of Magnetic Field Structures on Different Scales in and around the Filamentary Dark Cloud GF 9","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Magnetic field; Polarization (electrochemistry); Polarimetry; Saturation (graph theory); Protein filament; Faraday effect; Linear polarization","score_opus":0.009663213061015122,"score_gpt":0.25620677963942473,"score_spread":0.24654356657840962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992865401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99896955,0.000022012544,0.00007444014,0.000014391312,0.0000017698079,0.000001878753,0.00017317757,0.000009144482,0.0007336396],"genre_scores_gemma":[0.9994211,0.000017858936,0.0000949812,0.0000043134423,0.000004906208,0.0000015324094,0.00037241192,0.0000031009859,0.00007985239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999461,0.0000034737468,0.0000025204145,0.000014498425,0.000011356418,0.000022087586],"domain_scores_gemma":[0.9996984,0.000043871365,0.000083862826,0.000016989186,0.000059567206,0.000097328884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006633095,0.00014248783,0.00014452146,0.0014384682,0.00028153195,0.00038167922,0.00020337482,0.00019077497,0.00080582406],"category_scores_gemma":[0.0003732428,0.00009949569,0.00014981726,0.00065779,0.00031308798,0.00023573224,0.00034544713,0.00024567754,0.00010301044],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011795065,0.00011992419,0.80061096,0.0000627293,0.00016387847,0.0013108714,0.0010408631,0.0028047615,0.17024817,0.0008302799,0.00068643957,0.020941604],"study_design_scores_gemma":[0.0000047623607,0.000014978996,0.9984957,0.0000024508806,0.000008119271,0.000056186,0.0000811559,0.0005613547,0.00060769945,0.000031419295,0.00013299029,0.0000031174472],"about_ca_topic_score_codex":0.008846854,"about_ca_topic_score_gemma":0.008880605,"teacher_disagreement_score":0.008846854,"about_ca_system_score_codex":0.0003939271,"about_ca_system_score_gemma":0.00009006645,"threshold_uncertainty_score":0.017590702},"labels":[],"label_agreement":null},{"id":"W1992868229","doi":"10.1086/382498","title":"A Study of the Reionization History of Intergalactic Helium with<i>FUSE</i>and the Very Large Telescope","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Quasar; Reionization; Astrophysics; Redshift; Intergalactic travel; Absorption (acoustics); Spectral line; Astronomy; Absorption spectroscopy; Ionization; Telescope; Emission spectrum; Galaxy; Optics","score_opus":0.00538533120964078,"score_gpt":0.18731016121942362,"score_spread":0.18192483000978285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992868229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950801,0.00071355444,0.0005009055,0.00011892522,0.0000075525986,0.00000477981,0.0003205312,0.000016878124,0.0032366975],"genre_scores_gemma":[0.9983236,0.00020097972,0.00030345007,0.000032766417,0.000009031834,0.0000019233516,0.0003816375,0.000014229357,0.0007322236],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985707,0.000032146923,0.0000067623605,0.000039192764,0.000028757016,0.00003606061],"domain_scores_gemma":[0.9986519,0.0005386246,0.00034481013,0.00012961913,0.00017830555,0.00015672059],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096036016,0.00024001961,0.00030719637,0.000872708,0.00062935025,0.00067131175,0.00040095532,0.00051414757,0.0010119395],"category_scores_gemma":[0.0015847379,0.00025867735,0.0003718802,0.0016447713,0.00033339064,0.0015084845,0.00046085578,0.0005117725,0.00019217911],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012687488,0.00030910247,0.89443356,0.00017237218,0.0005285407,0.0010538076,0.0014317869,0.0117557105,0.047658157,0.007227192,0.0017111064,0.032449935],"study_design_scores_gemma":[0.000023818713,0.00014713583,0.9824814,0.000020967986,0.00007787142,0.00025978388,0.00028042414,0.008152671,0.0049442844,0.0008628039,0.0027154717,0.000033463602],"about_ca_topic_score_codex":0.012681477,"about_ca_topic_score_gemma":0.016317388,"teacher_disagreement_score":0.012681477,"about_ca_system_score_codex":0.0011558479,"about_ca_system_score_gemma":0.00028071555,"threshold_uncertainty_score":0.025215328},"labels":[],"label_agreement":null},{"id":"W1992870031","doi":"10.1086/374550","title":"<i>Far Ultraviolet Spectroscopic Explorer</i>Snapshot Survey of O<scp>vi</scp>Variability in the Winds of 66 OB‐Type Stars","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Stars; Astrophysics; Spectral line; Galaxy; Wind speed; Stellar classification; Atmospheric sciences; Astronomy; Meteorology","score_opus":0.02167607108846969,"score_gpt":0.24572351927727276,"score_spread":0.22404744818880307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1992870031","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99543214,0.00008925045,0.0004275214,0.000028409173,0.000004443688,0.000014701691,0.0031911638,0.000043199794,0.000769329],"genre_scores_gemma":[0.9831457,0.00015906413,0.0048311907,0.00005150437,0.000019032881,0.000022069455,0.010667603,0.000021382086,0.0010825545],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984777,0.000022888473,0.000011097725,0.00003550605,0.000042765743,0.00003989259],"domain_scores_gemma":[0.9993431,0.00003788371,0.00016185304,0.00006223907,0.00010801414,0.00028685483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033611766,0.00019800816,0.00017643599,0.0009989796,0.00035559316,0.00035006844,0.00017067055,0.00017570118,0.00088827626],"category_scores_gemma":[0.0003431004,0.00014755737,0.00020429115,0.0007458637,0.00008531737,0.00022595667,0.0004959752,0.00025522045,0.00037288447],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001454309,0.00010943624,0.9498145,0.000025079498,0.00008980954,0.00026013286,0.00027849106,0.0003838446,0.03211218,0.000058232883,0.0011486541,0.015574184],"study_design_scores_gemma":[0.0000032873888,0.00007405967,0.9977927,0.0000026268758,0.000009092445,0.000101299716,0.00006663245,0.00023115207,0.0009903968,0.000009707967,0.000715459,0.0000035680869],"about_ca_topic_score_codex":0.008415309,"about_ca_topic_score_gemma":0.020490458,"teacher_disagreement_score":0.008415309,"about_ca_system_score_codex":0.00015107737,"about_ca_system_score_gemma":0.00022138389,"threshold_uncertainty_score":0.016732633},"labels":[],"label_agreement":null},{"id":"W1993011209","doi":"10.1088/0004-637x/711/2/1033","title":"LoCuSS: A COMPARISON OF CLUSTER MASS MEASUREMENTS FROM<i>XMM-NEWTON</i>AND SUBARU—TESTING DEVIATION FROM HYDROSTATIC EQUILIBRIUM AND NON-THERMAL PRESSURE SUPPORT","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Max-Planck-Gesellschaft; Space Telescope Science Institute; Bundesministerium für Bildung und Forschung; University of Maryland, Baltimore County; National Aeronautics and Space Administration","keywords":"Hydrostatic equilibrium; Physics; Cluster (spacecraft); RADIUS; Astrophysics; Adiabatic process; Subaru Telescope; Thermodynamics","score_opus":0.022877116411493047,"score_gpt":0.2526210545537874,"score_spread":0.22974393814229438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993011209","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979127,0.000164036,0.00045364894,0.000018842717,0.000004576676,0.0000063066823,0.00045226814,0.00011411973,0.0008735048],"genre_scores_gemma":[0.997212,0.000041937823,0.0010880055,0.0000135576365,0.000009394504,0.000008261971,0.0014274424,0.00004149305,0.00015802661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99940073,0.00008812725,0.00004579876,0.00017861801,0.00021248443,0.00007422935],"domain_scores_gemma":[0.99777514,0.00021989067,0.00096838764,0.00031182324,0.00033844833,0.0003863436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001116036,0.00032932532,0.00040823515,0.003516282,0.00034313803,0.00095198717,0.0007492836,0.00036151748,0.0006605992],"category_scores_gemma":[0.002756178,0.00030825488,0.00036365056,0.001438997,0.00040718805,0.00064695015,0.0014646532,0.00019187701,0.00057941285],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032363343,0.0000265578,0.97964513,0.000026423448,0.00020884327,0.00010086681,0.0004981884,0.0008449873,0.008051296,0.0002483957,0.00047173855,0.009553962],"study_design_scores_gemma":[0.000009888966,0.000030164085,0.99646795,0.0000050233934,0.000022093302,0.00010054638,0.00012578574,0.0016330174,0.0011753169,0.000066135784,0.0003566872,0.0000073921324],"about_ca_topic_score_codex":0.0032246981,"about_ca_topic_score_gemma":0.0046535637,"teacher_disagreement_score":0.003516282,"about_ca_system_score_codex":0.00041647526,"about_ca_system_score_gemma":0.00014832887,"threshold_uncertainty_score":0.0064118505},"labels":[],"label_agreement":null},{"id":"W1993059472","doi":"10.1086/322329","title":"Evidence for an Accelerating Wind as the Broad‐Line Region in NGC 3516","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Emission spectrum; Flux (metallurgy); Active galactic nucleus; Line (geometry); Hubble sequence; Ionization; Wavelength","score_opus":0.05494797485999368,"score_gpt":0.2915814677056509,"score_spread":0.23663349284565724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993059472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99957556,0.000039557406,0.000036936704,0.0000047671842,6.519377e-7,0.000001505326,0.00004210061,0.000003658244,0.00029533968],"genre_scores_gemma":[0.9994925,0.00003615657,0.000102310776,0.0000034908471,0.000001138539,0.0000018773895,0.00012615249,0.0000011566979,0.00023522132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999577,0.000003802379,0.00000405368,0.000011976367,0.000009058358,0.00001337358],"domain_scores_gemma":[0.9997193,0.000016790904,0.00012756312,0.000027840311,0.000036137917,0.00007236049],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009513753,0.00016907122,0.00011536467,0.0004083663,0.00026232086,0.00038190724,0.00014425463,0.00013263559,0.00092916045],"category_scores_gemma":[0.00023742896,0.00012790265,0.00007368171,0.00038522226,0.00031473668,0.00015072168,0.0002580389,0.00013415482,0.0001379541],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021845975,0.00004927865,0.79928905,0.00003452042,0.00003106336,0.0006911878,0.00081968337,0.00051527505,0.19088446,0.00069792615,0.00016626772,0.00660278],"study_design_scores_gemma":[0.000012348695,0.0000926654,0.99596643,0.0000085658385,0.000013149005,0.0005145376,0.00015751451,0.00031267956,0.0019836444,0.00019363382,0.00073899946,0.0000058405026],"about_ca_topic_score_codex":0.0070026717,"about_ca_topic_score_gemma":0.014954255,"teacher_disagreement_score":0.0070026717,"about_ca_system_score_codex":0.0002138329,"about_ca_system_score_gemma":0.00013746864,"threshold_uncertainty_score":0.013923824},"labels":[],"label_agreement":null},{"id":"W1993072277","doi":"10.1088/0004-637x/740/1/31","title":"FAR-INFRARED LUMINOUS SUPERNOVA REMNANT Kes 17","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Supernova; Infrared; Spectral energy distribution; Emission spectrum; Luminosity; Line (geometry); Far infrared; Supernova remnant; Molecular cloud; Astronomy; Spectral line; Galaxy; Stars","score_opus":0.01731113640299962,"score_gpt":0.21291150686489033,"score_spread":0.19560037046189072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993072277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985092,0.0001445973,0.00010720777,0.0000031225031,0.000002888934,0.0000027683902,0.00022840998,0.000025819387,0.0009758982],"genre_scores_gemma":[0.9972253,0.00013773023,0.00038399934,0.000012778072,0.000008841848,0.000005601268,0.0018703206,0.000013323664,0.00034230237],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998815,0.000007959727,0.000009194763,0.000038723658,0.000025083073,0.000037624464],"domain_scores_gemma":[0.99969554,0.000021858177,0.00009651595,0.000043633652,0.00003682264,0.00010565828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024110217,0.00048528696,0.00045337126,0.00063788786,0.00027124875,0.0005576411,0.00020691927,0.0001715542,0.00092246226],"category_scores_gemma":[0.00021233961,0.00016404838,0.00036451255,0.00036452594,0.00022666053,0.00018324004,0.0005209034,0.00022967963,0.0004619547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012481642,0.00019797418,0.76747465,0.00014571137,0.00033676258,0.0024371792,0.00043219753,0.0012149836,0.21376556,0.00055804354,0.0006809593,0.011507733],"study_design_scores_gemma":[0.000027179596,0.00042937492,0.9739463,0.000018687837,0.000108195854,0.002074541,0.00025619473,0.0012498603,0.018363342,0.00012224715,0.0033848356,0.000019142759],"about_ca_topic_score_codex":0.0012194314,"about_ca_topic_score_gemma":0.0016919296,"teacher_disagreement_score":0.0012194314,"about_ca_system_score_codex":0.00018959644,"about_ca_system_score_gemma":0.00010130792,"threshold_uncertainty_score":0.0030859709},"labels":[],"label_agreement":null},{"id":"W1993076795","doi":"10.1086/426049","title":"Tramp Novae between Galaxies in the Fornax Cluster: Tracers of Intracluster Light","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Astronomy; Intracluster medium; Virgo Cluster; Observatory; Galaxy cluster; Galaxy; Cluster (spacecraft)","score_opus":0.010977912284473604,"score_gpt":0.23600212272646529,"score_spread":0.22502421044199167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993076795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993118,0.00013274366,0.00015947723,0.000007235186,0.0000010764569,0.0000022118786,0.000053396838,0.00000560606,0.0003263889],"genre_scores_gemma":[0.998988,0.00007209279,0.0004742771,0.000004344593,0.000004890113,0.0000036929373,0.00021000768,0.0000033695005,0.00023936924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998,0.000033931065,0.000008902921,0.00006352666,0.000038193193,0.00005545361],"domain_scores_gemma":[0.99699926,0.0006604628,0.0013620612,0.0002597403,0.00020954823,0.00050895585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046778936,0.0001765851,0.00021286747,0.0016116214,0.0005682917,0.0007768532,0.0002590545,0.00027304736,0.00083002966],"category_scores_gemma":[0.0020661494,0.00016331983,0.0001699121,0.0010358578,0.00041924402,0.0006189358,0.0008107836,0.00036678233,0.00014953752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000053607182,0.000016649818,0.9909882,0.000008488929,0.000022529392,0.000053689506,0.00034752578,0.00016804642,0.0028086726,0.00015320335,0.000044113945,0.0053352],"study_design_scores_gemma":[0.0000013253613,0.000028962317,0.9985833,0.0000028602178,0.0000069000207,0.00012342396,0.00013170856,0.0003352376,0.00042395992,0.000079068515,0.00028033642,0.0000028558975],"about_ca_topic_score_codex":0.004294318,"about_ca_topic_score_gemma":0.009337329,"teacher_disagreement_score":0.004294318,"about_ca_system_score_codex":0.00040519275,"about_ca_system_score_gemma":0.000165127,"threshold_uncertainty_score":0.008538604},"labels":[],"label_agreement":null},{"id":"W1993096612","doi":"10.1086/367618","title":"A Critical Examination of Halo White Dwarf Candidates","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Galactic halo; Proper motion; Halo; Stars; Supernova; Population; Photometry (optics); Gravitational microlensing","score_opus":0.009816095381969493,"score_gpt":0.2344960429182422,"score_spread":0.2246799475362727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993096612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98408854,0.0012521689,0.0020477306,0.00036737783,0.000024394903,0.000038590857,0.0012509967,0.00009152884,0.01083866],"genre_scores_gemma":[0.9898241,0.00071209605,0.001847189,0.00009171484,0.000029710382,0.000019202249,0.0015068089,0.000029119925,0.005939887],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998185,0.000022471777,0.000012703531,0.000028036036,0.00006972405,0.00004854404],"domain_scores_gemma":[0.99929893,0.00020702573,0.00009772771,0.000051048824,0.00019278142,0.00015258107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040480957,0.00020357386,0.00023507686,0.0024176352,0.0007229087,0.0005040908,0.00018257192,0.000103841136,0.0050357217],"category_scores_gemma":[0.0012347273,0.00007487478,0.00019370975,0.00080282456,0.00011710546,0.00027226153,0.00043871507,0.00011042391,0.00080652273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004243496,0.000044837583,0.8292124,0.00017089347,0.000056429006,0.0032501128,0.0010774324,0.0014166208,0.015797457,0.0043999148,0.0057975585,0.13835196],"study_design_scores_gemma":[0.000010555337,0.0001381988,0.9523691,0.000057598187,0.000056672015,0.004237755,0.001650008,0.0023240403,0.0038292417,0.0016912629,0.033618513,0.000016996253],"about_ca_topic_score_codex":0.0040744967,"about_ca_topic_score_gemma":0.0109708505,"teacher_disagreement_score":0.0050357217,"about_ca_system_score_codex":0.00022201486,"about_ca_system_score_gemma":0.00033946696,"threshold_uncertainty_score":0.01684618},"labels":[],"label_agreement":null},{"id":"W1993177046","doi":"10.1086/518366","title":"Laboratory Simulation of 11-15 μm Spectra Associated with Polycyclic Aromatic Hydrocarbon Molecules","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Carbon Nanotubes in Composites","field":"Materials Science","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Coronene; Polycyclic aromatic hydrocarbon; Carbon fibers; Spectral line; Molecule; Physics; Astrochemistry; Amorphous carbon; Interstellar medium; Hydrocarbon; Astrophysics; Ring (chemistry); Amorphous solid; Analytical Chemistry (journal); Chemical physics; Crystallography; Materials science; Chemistry; Astrobiology; Organic chemistry; Composite number; Galaxy; Astronomy","score_opus":0.006534820917169375,"score_gpt":0.23430976382827212,"score_spread":0.22777494291110276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993177046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947702,0.000033696746,0.002573219,0.00006643853,0.000008492299,0.000012668159,0.00014270691,0.000065682725,0.0023267556],"genre_scores_gemma":[0.9974655,0.000028382952,0.0019284447,0.000014465313,0.0000032049068,0.000019816196,0.00016538626,0.000013924496,0.00036090592],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999373,0.000008690732,0.0000016503085,0.000012337892,0.000016757256,0.000023234172],"domain_scores_gemma":[0.9996836,0.00016817621,0.00004023616,0.000022589475,0.00005389638,0.000031547374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017299976,0.0002474017,0.00024812124,0.0001830518,0.00033622407,0.00028041488,0.0004804731,0.0005530089,0.0016548967],"category_scores_gemma":[0.00061332836,0.00019440269,0.00034385239,0.000220406,0.0003992057,0.0003066755,0.00020437084,0.00045744606,0.00011412695],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022968047,0.00030546548,0.0100532025,0.00007808436,0.000058714904,0.00045756993,0.0001279162,0.93578374,0.046896532,0.002387795,0.0006018633,0.0030194127],"study_design_scores_gemma":[0.00004288253,0.0001395448,0.003206907,0.0000041294297,0.000012415024,0.000028468237,0.00003873619,0.9830526,0.012877803,0.0003190276,0.00026541884,0.000011989869],"about_ca_topic_score_codex":0.0049759597,"about_ca_topic_score_gemma":0.0030679244,"teacher_disagreement_score":0.0049759597,"about_ca_system_score_codex":0.00058789284,"about_ca_system_score_gemma":0.00032006108,"threshold_uncertainty_score":0.009894013},"labels":[],"label_agreement":null},{"id":"W1993196791","doi":"10.1086/432157","title":"Internal Alignment of the Halos of Disk Galaxies in Cosmological Hydrodynamic Simulations","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":168,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; University of Victoria","funders":"","keywords":"Halo; Dark matter halo; Galaxy; Dark matter; Galactic halo; Thick disk; Galaxy formation and evolution","score_opus":0.006865023223574803,"score_gpt":0.2187982454528284,"score_spread":0.2119332222292536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993196791","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99744093,0.00004539604,0.0010159967,0.00004627206,0.0000044184258,0.000008918581,0.00021506393,0.00006306037,0.0011600888],"genre_scores_gemma":[0.9977229,0.000044063865,0.0012627267,0.000019021905,0.0000038390926,0.00001362044,0.00063815416,0.000055442837,0.0002403094],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999795,0.00007002174,0.000013065818,0.00003180244,0.000035969726,0.00005401704],"domain_scores_gemma":[0.99872655,0.0004683928,0.00013850386,0.00014540159,0.00020147409,0.0003197845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069697486,0.00037965918,0.0005977021,0.00069205544,0.0007248859,0.00093029655,0.00072320225,0.00051601965,0.0010285185],"category_scores_gemma":[0.0033458315,0.00041450103,0.00063590053,0.00070964976,0.00061739684,0.0004623816,0.0007149589,0.00063204113,0.00013610744],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019326089,0.00009871158,0.05435962,0.00003420636,0.00017348824,0.00011501285,0.00019023544,0.93571705,0.003174191,0.0025941767,0.00059560174,0.0027543076],"study_design_scores_gemma":[0.0000646032,0.00005710387,0.020784773,0.000009554717,0.000049702772,0.000025454105,0.00008293617,0.9763897,0.0011953589,0.00086759846,0.00044449494,0.00002879076],"about_ca_topic_score_codex":0.02986992,"about_ca_topic_score_gemma":0.024097398,"teacher_disagreement_score":0.02986992,"about_ca_system_score_codex":0.00170547,"about_ca_system_score_gemma":0.00086783915,"threshold_uncertainty_score":0.059392095},"labels":[],"label_agreement":null},{"id":"W1993241454","doi":"10.1086/504066","title":"AmFm Stars as a Test of Rotational Mixing Models","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Stars; Astrophysics; Supergiant; Turbulence; Stellar evolution; Radiative transfer; Angular momentum; Diffusion; Abundance (ecology); Anisotropy; Classical mechanics; Mechanics; Thermodynamics","score_opus":0.010622648883411669,"score_gpt":0.21898494808395103,"score_spread":0.20836229920053936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993241454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98932517,0.00010361236,0.004025854,0.00027926985,0.000036616722,0.000010024757,0.00028449128,0.00014782936,0.005787171],"genre_scores_gemma":[0.99839336,0.000015320962,0.0008188869,0.000056152814,0.00001737116,0.000004645694,0.00033929362,0.000030721352,0.00032424997],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992112,0.00029305185,0.000031060983,0.00020349467,0.00014602867,0.000115148956],"domain_scores_gemma":[0.9954899,0.0020034683,0.0006396445,0.0006570815,0.0003519577,0.00085789163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0036422005,0.0005951571,0.0006794857,0.0007819169,0.0009082889,0.0017451986,0.0006904303,0.0013267606,0.0027107103],"category_scores_gemma":[0.0054535405,0.00016116916,0.0006548935,0.00070318364,0.00068396534,0.0008610914,0.0011174025,0.0008263537,0.00057317177],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.009323791,0.0010935742,0.64550525,0.0003658567,0.0010009948,0.0013498123,0.0012316575,0.049534436,0.087846726,0.13778777,0.008133553,0.05682659],"study_design_scores_gemma":[0.001309434,0.0029734897,0.419743,0.00009104598,0.00045031647,0.001305485,0.0021049576,0.4346924,0.027871562,0.1008245,0.008486376,0.00014742817],"about_ca_topic_score_codex":0.0011001382,"about_ca_topic_score_gemma":0.0005605988,"teacher_disagreement_score":0.0036422005,"about_ca_system_score_codex":0.0005708234,"about_ca_system_score_gemma":0.00029298628,"threshold_uncertainty_score":0.019262016},"labels":[],"label_agreement":null},{"id":"W1993261306","doi":"10.1088/0004-637x/738/1/66","title":"SIMULATIONS OF TURBULENT DYNAMOS DRIVEN BY THE MAGNETIC HELICITY FLUX","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Dynamo; Physics; Magnetic helicity; Helicity; Magnetohydrodynamic turbulence; Turbulence; Solar dynamo; Dynamo theory; Magnetic field; Magnetohydrodynamics; Classical mechanics; Electromotive force; Mechanics; Quantum mechanics","score_opus":0.009961452954764938,"score_gpt":0.21642439669134633,"score_spread":0.2064629437365814,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993261306","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898627,0.00010778425,0.0046882774,0.00025295618,0.000057227357,0.000046337587,0.00057034515,0.00015023061,0.0042642066],"genre_scores_gemma":[0.99492526,0.00005416768,0.003600146,0.000043357544,0.000012792542,0.00007376379,0.000526657,0.000043835542,0.000719943],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983,0.000046314864,0.000012032201,0.000026327176,0.000033551834,0.00005169828],"domain_scores_gemma":[0.9987453,0.00070219283,0.00012243862,0.00006694894,0.00014229593,0.00022083428],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004265566,0.00051288697,0.0008131933,0.00045406635,0.00066861504,0.0006681421,0.0009831064,0.0009800429,0.0021354884],"category_scores_gemma":[0.0019632017,0.00036225512,0.0004818966,0.0005699557,0.00093358144,0.0005231862,0.0006037201,0.0010477353,0.00012565643],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004090922,0.00027337365,0.006940776,0.00007576464,0.0001035804,0.00028796247,0.00015582528,0.9805638,0.004522912,0.004240077,0.0007314299,0.0016953232],"study_design_scores_gemma":[0.000062687315,0.000053964653,0.0009819478,0.000007111032,0.000009251178,0.000011579234,0.000034278608,0.9971085,0.00079343416,0.00070708373,0.00022129116,0.000008978768],"about_ca_topic_score_codex":0.009337333,"about_ca_topic_score_gemma":0.0066178846,"teacher_disagreement_score":0.009337333,"about_ca_system_score_codex":0.00076257763,"about_ca_system_score_gemma":0.00086701347,"threshold_uncertainty_score":0.018565953},"labels":[],"label_agreement":null},{"id":"W1993317195","doi":"10.1088/0004-637x/787/2/138","title":"HYDROGEN-POOR SUPERLUMINOUS SUPERNOVAE AND LONG-DURATION GAMMA-RAY BURSTS HAVE SIMILAR HOST GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":249,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency; Planetary Science Division; Science Mission Directorate; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Aeronautics and Space Administration; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Galaxy; Supernova; Redshift; Photometry (optics); Star formation; Stars; Metallicity; Magnetar","score_opus":0.008923664303022341,"score_gpt":0.2174374089607426,"score_spread":0.20851374465772027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993317195","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992588,0.00010403535,0.000057529553,0.0000047825097,7.7978723e-7,0.0000028473041,0.00011035476,0.0000056325516,0.0004551116],"genre_scores_gemma":[0.9992811,0.000049548304,0.00007622106,0.0000063946745,0.0000026876037,0.000002566778,0.00043980652,0.0000017002149,0.00014001055],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997497,0.000028757879,0.000026934595,0.000083714986,0.000039423852,0.00007142456],"domain_scores_gemma":[0.9989698,0.00010467554,0.0005145789,0.00009914451,0.00007485306,0.0002369361],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022458076,0.00026332767,0.00029083443,0.0012133064,0.00031913575,0.0006852624,0.00026044206,0.00020662925,0.0020937885],"category_scores_gemma":[0.00064191263,0.00017930027,0.00021409648,0.00066789985,0.00028176315,0.0003108143,0.00058693375,0.00015056094,0.00031037015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000078366545,0.000016823476,0.99492764,0.000007252744,0.00003375808,0.000047062436,0.000055708166,0.00005341984,0.003425299,0.000047630776,0.00002272516,0.0012842643],"study_design_scores_gemma":[0.0000024317837,0.000022073304,0.99923754,0.0000011630143,0.000006731874,0.00020589528,0.00007493197,0.00006565788,0.00024887398,0.000022676697,0.00011110724,8.8820195e-7],"about_ca_topic_score_codex":0.002435232,"about_ca_topic_score_gemma":0.0036446205,"teacher_disagreement_score":0.002435232,"about_ca_system_score_codex":0.00017683886,"about_ca_system_score_gemma":0.00010208489,"threshold_uncertainty_score":0.00700444},"labels":[],"label_agreement":null},{"id":"W1993373838","doi":"10.1088/0004-637x/730/1/42","title":"DISCOVERY OF AN ∼23<i>M</i><sub>Jup</sub>BROWN DWARF ORBITING ∼700 AU FROM THE MASSIVE STAR HIP 78530 IN UPPER SCORPIUS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Brown dwarf; Proper motion; Physics; Astrophysics; Surface gravity; Luminosity; Stellar classification; Stars; Subdwarf; Spectral line; Astronomy; White dwarf","score_opus":0.01672008173448288,"score_gpt":0.21283201315064787,"score_spread":0.19611193141616498,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993373838","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999403,0.000033855384,0.000047826183,0.000012086749,0.0000014306953,0.0000012799279,0.00003546035,0.000008583811,0.0004565659],"genre_scores_gemma":[0.99928504,0.00003141224,0.00018535159,0.00001577673,0.000005111468,0.0000012415976,0.00017466606,0.0000025124195,0.00029890946],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995756,0.0000019193733,0.000002206372,0.000014448059,0.000011286411,0.000012522739],"domain_scores_gemma":[0.99984825,0.000010096133,0.00006500534,0.000013649596,0.000013984592,0.000049138947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007350878,0.00013470718,0.00012213126,0.00042714254,0.00049278815,0.00036415952,0.00024808434,0.00032292472,0.00081564224],"category_scores_gemma":[0.00017306476,0.000116443465,0.00009720379,0.0002493832,0.00036433485,0.00017689199,0.00046081364,0.00019402399,0.00029807436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024369975,0.000071504386,0.7437167,0.000055755267,0.000039124785,0.010795933,0.001100878,0.00017990502,0.2215839,0.00027508044,0.00055960217,0.021377861],"study_design_scores_gemma":[0.000004451447,0.00011415549,0.9858856,0.0000054081675,0.000018270608,0.0055087395,0.00023387562,0.00015877088,0.0065115467,0.000067450346,0.0014869308,0.0000047962853],"about_ca_topic_score_codex":0.003869244,"about_ca_topic_score_gemma":0.007029604,"teacher_disagreement_score":0.003869244,"about_ca_system_score_codex":0.00032919348,"about_ca_system_score_gemma":0.0001661338,"threshold_uncertainty_score":0.00769341},"labels":[],"label_agreement":null},{"id":"W1993433815","doi":"10.1088/0004-637x/761/1/67","title":"TWO-STAGE FRAGMENTATION FOR CLUSTER FORMATION: ANALYTICAL MODEL AND OBSERVATIONAL CONSIDERATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Fragmentation (computing); Molecular cloud; Cluster (spacecraft); Star formation; Planar; Star cluster; Ionization","score_opus":0.06156751467521352,"score_gpt":0.31502472499098977,"score_spread":0.2534572103157762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993433815","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.46199328,0.0035556138,0.45444363,0.0036671802,0.000117050986,0.00027494607,0.00084277435,0.0009297332,0.07417571],"genre_scores_gemma":[0.966088,0.0015027336,0.020350544,0.0001625263,0.00013818365,0.00023957262,0.00019016604,0.00010500895,0.01122319],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99988365,0.000031645057,0.0000042195416,0.000014128985,0.00002538814,0.000040965962],"domain_scores_gemma":[0.99929965,0.0002790688,0.0001387554,0.00007429124,0.00012856552,0.00007970408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060015044,0.00056543277,0.00044265226,0.0009077031,0.000700819,0.0011740336,0.0019321193,0.0009750229,0.00362445],"category_scores_gemma":[0.0027363277,0.00031077786,0.0007956086,0.00090558804,0.00089832017,0.0015525705,0.0009790238,0.0005802327,0.0009864889],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000615842,0.00012607356,0.007632793,0.00013802912,0.000040133225,0.0009958424,0.0006196342,0.5826813,0.0021989592,0.3936577,0.0040632416,0.0077847205],"study_design_scores_gemma":[0.00001243265,0.000016099253,0.0010770692,0.000011134082,0.000007383276,0.00013976547,0.00005403712,0.9337367,0.00010224484,0.06390677,0.00092312304,0.000013205414],"about_ca_topic_score_codex":0.010273009,"about_ca_topic_score_gemma":0.0041568084,"teacher_disagreement_score":0.010273009,"about_ca_system_score_codex":0.0020075897,"about_ca_system_score_gemma":0.0008532672,"threshold_uncertainty_score":0.020426452},"labels":[],"label_agreement":null},{"id":"W1993509986","doi":"10.1088/0004-637x/704/2/1262","title":"INFLUENCE OF THERMOHALINE CONVECTION ON DIFFUSION-INDUCED IRON ACCUMULATION IN A STARS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Moncton","funders":"","keywords":"Stars; Convection; Thermohaline circulation; Convection zone; Diffusion; Opacity","score_opus":0.016442002789982507,"score_gpt":0.26272309082527834,"score_spread":0.24628108803529583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993509986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984491,0.00016068915,0.00042099878,0.000036804482,0.0000069937314,0.000004181663,0.000054877495,0.000043655164,0.0008227312],"genre_scores_gemma":[0.99968624,0.00004097241,0.00014664068,0.0000069882135,0.0000032604225,0.000001599901,0.000024564846,0.000011478011,0.000078343626],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989486,0.000024846373,0.000012332664,0.000024497396,0.000014089181,0.000029414432],"domain_scores_gemma":[0.99936455,0.0003119979,0.00009679984,0.0000619636,0.00006514533,0.000099501645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027100937,0.00053889374,0.00043338788,0.0003687448,0.0004025286,0.0008808085,0.00024945528,0.00045603307,0.000982576],"category_scores_gemma":[0.0014102979,0.00024568106,0.000728404,0.0002644619,0.00063257053,0.00041692567,0.00069110934,0.0003151748,0.00013437298],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002790028,0.00032843667,0.2278653,0.00031947024,0.000421959,0.0024057338,0.00039952123,0.32141647,0.42065024,0.0028155574,0.00046398275,0.020123264],"study_design_scores_gemma":[0.00044392608,0.00075870386,0.276645,0.00005951879,0.00025513445,0.0006547976,0.00027658397,0.6273454,0.09095429,0.0015667636,0.0009306425,0.00010916988],"about_ca_topic_score_codex":0.0038489192,"about_ca_topic_score_gemma":0.001205755,"teacher_disagreement_score":0.0038489192,"about_ca_system_score_codex":0.00040743095,"about_ca_system_score_gemma":0.00027742222,"threshold_uncertainty_score":0.007652998},"labels":[],"label_agreement":null},{"id":"W1993535337","doi":"10.1086/375716","title":"Neutral Hydrogen Associated with NGC 7129","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Star formation; Context (archaeology); Astronomy; Interstellar medium; Photodissociation; Line (geometry); Galaxy; Stars; Photochemistry","score_opus":0.008892058380060961,"score_gpt":0.2154644694995089,"score_spread":0.20657241111944794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993535337","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99642247,0.0001645711,0.000099701545,0.000012013467,0.000003356459,0.0000037925658,0.00019967016,0.000012823407,0.0030815338],"genre_scores_gemma":[0.99857914,0.00006483249,0.00016523823,0.000008353634,0.0000023142295,0.00000205607,0.0005458489,0.000002284948,0.00062998506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999238,0.000004953501,0.0000033390024,0.0000142147,0.000032217573,0.000021486003],"domain_scores_gemma":[0.9998777,0.000006989005,0.000035425768,0.0000113553815,0.000025444904,0.0000431488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004522421,0.00014124572,0.00010661729,0.00039408356,0.00062332145,0.00026854532,0.00017221076,0.00016171673,0.0010568454],"category_scores_gemma":[0.00016405087,0.00006801491,0.000052629835,0.00054641627,0.00017926148,0.00009520896,0.000357671,0.00010409276,0.00044135159],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002903573,0.00008209704,0.64007837,0.00009850526,0.000043795357,0.0046568816,0.0015315491,0.0007171706,0.32548162,0.0011271954,0.0018218793,0.024070567],"study_design_scores_gemma":[0.000007838711,0.000075354146,0.98344857,0.00000839483,0.000008779191,0.0023121138,0.00037287376,0.00023371413,0.0035488687,0.00017703473,0.009796741,0.00000965096],"about_ca_topic_score_codex":0.017208422,"about_ca_topic_score_gemma":0.029215481,"teacher_disagreement_score":0.017208422,"about_ca_system_score_codex":0.00040923222,"about_ca_system_score_gemma":0.00017640472,"threshold_uncertainty_score":0.034216523},"labels":[],"label_agreement":null},{"id":"W1993554427","doi":"10.1086/424917","title":"Distances of Quasars and Quasar‐like Galaxies: Further Evidence That Quasi‐stellar Objects May Be Ejected from Active Galaxies","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Quasar; Astrophysics; Redshift; QSOS; Galaxy; Redshift survey; Astronomy; Asymmetry","score_opus":0.01582672078824259,"score_gpt":0.23475439589981392,"score_spread":0.21892767511157132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993554427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99687105,0.00030734582,0.0003564995,0.000086088054,0.0000024219398,0.0000017238136,0.00014807282,0.000010273204,0.0022165333],"genre_scores_gemma":[0.9993549,0.000053221655,0.00012218617,0.000022502245,0.000006127484,8.352254e-7,0.00013418245,0.0000029909772,0.00030308092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960285,0.000074627125,0.0000363682,0.000086162836,0.0001341313,0.00006580728],"domain_scores_gemma":[0.995001,0.0015166077,0.001618833,0.00053020957,0.0005686604,0.0007647063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069808896,0.00018656647,0.00016252721,0.0013137759,0.00043286168,0.0007926709,0.00045798754,0.00051105936,0.0025753938],"category_scores_gemma":[0.0037303076,0.00020236142,0.00016962831,0.00088717026,0.0007890971,0.00075950334,0.00079976686,0.00041730423,0.00042502396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000089922854,0.000025642728,0.9875107,0.00003179378,0.00005171804,0.00010648065,0.0003925965,0.00016962788,0.004598694,0.0010334094,0.00011331175,0.005875986],"study_design_scores_gemma":[0.0000030101276,0.000016070153,0.99896455,0.0000018745467,0.000007107886,0.00018271248,0.000060413346,0.0001038818,0.00025586438,0.00016682553,0.00023516433,0.0000024273227],"about_ca_topic_score_codex":0.0030071838,"about_ca_topic_score_gemma":0.00573251,"teacher_disagreement_score":0.0030071838,"about_ca_system_score_codex":0.0002488628,"about_ca_system_score_gemma":0.00016925398,"threshold_uncertainty_score":0.008615553},"labels":[],"label_agreement":null},{"id":"W1993673772","doi":"10.1086/588285","title":"The ACS LCID Project: RR Lyrae Stars as Tracers of Old Population Gradients in the Isolated Dwarf Spheroidal Galaxy Tucana","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"RR Lyrae variable; Metallicity; Dwarf spheroidal galaxy; Globular cluster; Hubble space telescope; Galaxy; Dwarf galaxy; Population","score_opus":0.01668676552148782,"score_gpt":0.27514449713852496,"score_spread":0.2584577316170371,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993673772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99182147,0.00042696143,0.00048998825,0.0001746069,0.000014170033,0.000013561756,0.0033669737,0.00010930905,0.003582932],"genre_scores_gemma":[0.9941287,0.00013357346,0.0009600532,0.00004540466,0.000015415986,0.000013802258,0.0034598918,0.000028099414,0.0012150211],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985826,0.000011995716,0.000004401717,0.000042688527,0.000033866738,0.000048725655],"domain_scores_gemma":[0.99942255,0.0000704981,0.00008542075,0.000056996872,0.00019358922,0.00017093332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052786845,0.00020880286,0.0002853718,0.0019160577,0.0011904847,0.0015725556,0.00066479476,0.00027182736,0.0009536826],"category_scores_gemma":[0.001241312,0.0001297821,0.00011075789,0.0023624406,0.00036593052,0.00027782534,0.0006250345,0.000221344,0.00015839543],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005745861,0.00019091032,0.91602933,0.00006977115,0.00010815377,0.00021995194,0.00078272703,0.0040863645,0.00942247,0.0018974467,0.006983369,0.05963492],"study_design_scores_gemma":[0.00003675976,0.000021852633,0.985427,0.000015658086,0.000057204204,0.000100818965,0.00036304607,0.005792078,0.002074305,0.00033099647,0.0057690297,0.0000112679045],"about_ca_topic_score_codex":0.42927322,"about_ca_topic_score_gemma":0.37081742,"teacher_disagreement_score":0.42927322,"about_ca_system_score_codex":0.003558378,"about_ca_system_score_gemma":0.0016736957,"threshold_uncertainty_score":0.8535491},"labels":[],"label_agreement":null},{"id":"W1993753822","doi":"10.1086/378954","title":"Thermal Stability of Rotating Low‐Mass Subgiants and Red Giants","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Red-giant branch; Red giant; Globular cluster; Astronomy; Stars; Horizontal branch; Red clump; Stellar evolution; Instability strip; Instability; Metallicity; Asymptotic giant branch; Thermonuclear fusion; Stellar rotation; Plasma; Cepheid variable; Mechanics","score_opus":0.012844700311613883,"score_gpt":0.22216510696206254,"score_spread":0.20932040665044865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993753822","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99948114,0.00006572833,0.00015682096,0.00000411791,5.1681565e-7,0.0000012543114,0.000044352713,0.0000068340496,0.00023941661],"genre_scores_gemma":[0.9996314,0.000029505338,0.00008007566,0.0000015137759,0.0000010906294,0.0000015422964,0.000108054264,0.0000034027203,0.0001433317],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995196,0.000006905486,0.000002559339,0.000016136479,0.0000071951563,0.000015365851],"domain_scores_gemma":[0.99980646,0.000035077697,0.000083546416,0.00001548169,0.000023304181,0.000036109817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018053647,0.00024507628,0.00022116974,0.00070236286,0.00027985135,0.00045061443,0.00025008968,0.00016943757,0.000809884],"category_scores_gemma":[0.0004502087,0.00012083432,0.00036690824,0.00032234154,0.00028701138,0.0001503479,0.00029160545,0.00015168737,0.00024763605],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074713875,0.00004018381,0.82148725,0.00009576564,0.00015895157,0.00025439006,0.0005251424,0.048652664,0.114227675,0.0017188574,0.0001987234,0.011893343],"study_design_scores_gemma":[0.0000218898,0.00026079096,0.92064655,0.000010455133,0.00006375635,0.00017810655,0.00017212737,0.06779357,0.009368405,0.00080454245,0.0006581681,0.000021658723],"about_ca_topic_score_codex":0.005756124,"about_ca_topic_score_gemma":0.002560542,"teacher_disagreement_score":0.005756124,"about_ca_system_score_codex":0.0006702119,"about_ca_system_score_gemma":0.00015641726,"threshold_uncertainty_score":0.011445224},"labels":[],"label_agreement":null},{"id":"W1993829695","doi":"10.1086/342645","title":"Multiresolution Analysis of Substructure in Dark Matter Halos","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Blind Source Separation Techniques","field":"Computer Science","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Halo; Substructure; Astrophysics; Dark matter; Physics; Population; Cluster analysis; Hierarchical clustering; Astronomy; Galaxy; Artificial intelligence; Computer science","score_opus":0.01272477731387269,"score_gpt":0.23870337105175274,"score_spread":0.22597859373788004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993829695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7009777,0.0007492176,0.2961201,0.00020768425,0.000021983149,0.000019290474,0.00008988292,0.00037012994,0.001444134],"genre_scores_gemma":[0.96202326,0.00028196152,0.03715895,0.000013602606,0.000018696039,0.000005748511,0.000069939095,0.00004447062,0.0003833821],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990284,0.000022983178,0.000004033233,0.000013013403,0.00003684918,0.000020229478],"domain_scores_gemma":[0.9996395,0.00013802537,0.00007744655,0.000054017957,0.000045006767,0.00004597685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041211693,0.00024944602,0.00028878424,0.0010586557,0.00028935916,0.00058112293,0.00021103311,0.00030316264,0.00048537948],"category_scores_gemma":[0.0016219257,0.00021966897,0.00033214546,0.0006603537,0.00038879094,0.00048196682,0.0006679517,0.00034532827,0.00011550822],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005379469,0.00009486103,0.01589742,0.00017467192,0.0001572231,0.0008629172,0.00066418195,0.6384006,0.15541346,0.028965387,0.001343978,0.1574873],"study_design_scores_gemma":[0.000022348231,0.00003318246,0.0110392915,0.000009115862,0.00001879243,0.00013985173,0.00006817474,0.96646136,0.009583835,0.01185347,0.00074791315,0.000022672366],"about_ca_topic_score_codex":0.00087189267,"about_ca_topic_score_gemma":0.00052119844,"teacher_disagreement_score":0.0010586557,"about_ca_system_score_codex":0.00021408626,"about_ca_system_score_gemma":0.00016593828,"threshold_uncertainty_score":0.0021795034},"labels":[],"label_agreement":null},{"id":"W1993847225","doi":"10.1088/0004-637x/777/2/144","title":"SMACK: A NEW ALGORITHM FOR MODELING COLLISIONS AND DYNAMICS OF PLANETESIMALS IN DEBRIS DISKS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"","keywords":"Planetesimal; Debris; Debris disk; Planet; Physics; Orbit (dynamics); Astrophysics; Planetary system; Meteorology; Aerospace engineering","score_opus":0.012285398340519638,"score_gpt":0.22889918905409973,"score_spread":0.21661379071358008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993847225","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01765683,0.00017525605,0.9765361,0.00009020325,0.000053407533,0.0000636605,0.0003856117,0.00360614,0.001432864],"genre_scores_gemma":[0.16712703,0.00021497568,0.8278313,0.00009983817,0.00004803811,0.0003147482,0.00097501837,0.0011590077,0.0022299725],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997527,0.000055653523,0.000021008978,0.00005249783,0.00008947548,0.000028626975],"domain_scores_gemma":[0.9992816,0.000320471,0.000090354544,0.000098137876,0.00013453483,0.00007507462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00073484174,0.0010996321,0.0008028544,0.00064175605,0.0009043033,0.001071072,0.0031838377,0.0013196027,0.0040125796],"category_scores_gemma":[0.002398841,0.0009125042,0.0009808742,0.00067611184,0.0006139044,0.002031542,0.0014155222,0.0013343684,0.001245036],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015990417,0.000039991257,0.0033964622,0.00010293536,0.00011726051,0.00015577974,0.00012360068,0.9356459,0.0027353251,0.013788113,0.0040494977,0.039685253],"study_design_scores_gemma":[0.0000110215815,0.0000052873656,0.000055593435,0.0000026653029,0.0000031392847,0.000014722592,0.0000043856166,0.9963721,0.00032722254,0.0020063743,0.0011937397,0.0000038501785],"about_ca_topic_score_codex":0.008373185,"about_ca_topic_score_gemma":0.007797056,"teacher_disagreement_score":0.008373185,"about_ca_system_score_codex":0.0007537338,"about_ca_system_score_gemma":0.0014697026,"threshold_uncertainty_score":0.016648889},"labels":[],"label_agreement":null},{"id":"W1993899320","doi":"10.1086/317159","title":"Continuum Pumping of Fe<scp>ii</scp>in the Orion Nebula","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Orion Nebula; Astrophysics; Spectral line; Emission spectrum; Nebula; Electron density; Electron; Stars; Computational physics; Astronomy","score_opus":0.00900124906558306,"score_gpt":0.23073004675313885,"score_spread":0.2217287976875558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993899320","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99755174,0.000049408904,0.0012300796,0.000080171725,0.0000047372037,0.0000037323853,0.000029834247,0.000055722827,0.0009944702],"genre_scores_gemma":[0.99897575,0.000025043986,0.0007580489,0.000016698186,0.0000022309669,0.0000042386077,0.000027036118,0.000011251236,0.00017952756],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.000013307652,0.000002563504,0.000010462922,0.000012781669,0.000014640316],"domain_scores_gemma":[0.9997304,0.00012720542,0.00004190715,0.00001869425,0.000034579025,0.000047114554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019300013,0.000317848,0.00026302482,0.00023438019,0.0005587531,0.0004970287,0.00055018096,0.0004692526,0.0010004939],"category_scores_gemma":[0.0009842278,0.00024039703,0.00028894318,0.0002140465,0.0005626944,0.00046391555,0.00044904544,0.00033053066,0.00009304739],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022343287,0.00015470573,0.030498259,0.000050559313,0.00007391075,0.0005200549,0.00020209458,0.9446572,0.015776819,0.0031508259,0.00028320975,0.0044089323],"study_design_scores_gemma":[0.00007834514,0.00008580045,0.008876914,0.000006904778,0.000018029865,0.00006185677,0.00006258544,0.98588145,0.0034491757,0.001161682,0.00030288927,0.000014379474],"about_ca_topic_score_codex":0.009943486,"about_ca_topic_score_gemma":0.0034043272,"teacher_disagreement_score":0.009943486,"about_ca_system_score_codex":0.0010663514,"about_ca_system_score_gemma":0.00044760996,"threshold_uncertainty_score":0.019771218},"labels":[],"label_agreement":null},{"id":"W1993917805","doi":"10.1086/424653","title":"The Crab Nebula’s Wisps in Radio and Optical","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Radio wave; Pulsar; Crab Pulsar; Radio astronomy; Radio frequency; Synchrotron; Striation","score_opus":0.00838119249770872,"score_gpt":0.2950839904786175,"score_spread":0.28670279798090875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993917805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.983093,0.0013065059,0.001134593,0.00014080007,0.000052524803,0.0000170921,0.0012397285,0.00015057888,0.01286521],"genre_scores_gemma":[0.9927516,0.0004341982,0.002717883,0.00011447353,0.000060541275,0.000011228087,0.0019915085,0.000048027156,0.0018704095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989164,0.0000052021683,0.0000049921055,0.000022672095,0.000039700397,0.000035810815],"domain_scores_gemma":[0.9995889,0.000038301834,0.00015800615,0.000050058883,0.0000895337,0.00007520535],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000135137,0.00019237326,0.00017492588,0.0018614437,0.00031646347,0.00089977385,0.00024733992,0.00029520213,0.0010107062],"category_scores_gemma":[0.0006031564,0.00024004432,0.00016582139,0.00093024294,0.00027977346,0.0003193238,0.0005292234,0.0004392417,0.00033311645],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001186371,0.00031744226,0.6328221,0.0005632895,0.00031063912,0.0066988296,0.002863034,0.0044979667,0.18696657,0.0016606529,0.010846331,0.15126672],"study_design_scores_gemma":[0.0000094022,0.000037605427,0.9867834,0.000027491025,0.000024595229,0.0012407051,0.00017280145,0.0005529045,0.0022585753,0.000096374606,0.008780182,0.000016040849],"about_ca_topic_score_codex":0.005252111,"about_ca_topic_score_gemma":0.014971939,"teacher_disagreement_score":0.005252111,"about_ca_system_score_codex":0.0003563688,"about_ca_system_score_gemma":0.0001494634,"threshold_uncertainty_score":0.010443091},"labels":[],"label_agreement":null},{"id":"W1993986614","doi":"10.1088/0004-637x/709/1/241","title":"A<i>CHANDRA X-RAY OBSERVATORY</i>STUDY OF PSR J1740-5340 AND CANDIDATE MILLISECOND PULSARS IN THE GLOBULAR CLUSTER NGC 6397","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; McGill University","funders":"","keywords":"Millisecond pulsar; Globular cluster; Pulsar; Pulsar planet; Observatory; Binary pulsar; Neutron star; Outflow; Cluster (spacecraft)","score_opus":0.011626337789086378,"score_gpt":0.2945704517342283,"score_spread":0.2829441139451419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1993986614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951906,0.00011389215,0.00004947341,0.00013062569,0.000014949775,0.000008647151,0.0015322276,0.000011630534,0.002947942],"genre_scores_gemma":[0.9901108,0.00017298889,0.00016826038,0.00013668413,0.000052296866,0.000011532235,0.0055226963,0.000022756716,0.0038019957],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998745,0.000006897119,0.0000104595965,0.000035948164,0.000036696565,0.000035484147],"domain_scores_gemma":[0.99924207,0.000093468276,0.00021923077,0.00009020256,0.00013785448,0.00021722949],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026654903,0.00017503381,0.0002893368,0.0017825891,0.0014958982,0.00089975074,0.0003277174,0.0003082437,0.009856244],"category_scores_gemma":[0.0005375904,0.00020072242,0.00025279072,0.0020205297,0.00045120288,0.0004387573,0.00054818025,0.00036378458,0.0012030429],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013364962,0.00026505167,0.9429986,0.000069280686,0.00017278538,0.0023987263,0.0008466219,0.00036410717,0.033639852,0.0007903509,0.004214646,0.012903613],"study_design_scores_gemma":[0.000016015036,0.000044819943,0.9977463,0.000004971528,0.00001997537,0.0002570144,0.0001064801,0.000054784137,0.0004981654,0.000048543738,0.0011990431,0.000003847705],"about_ca_topic_score_codex":0.033269234,"about_ca_topic_score_gemma":0.045657843,"teacher_disagreement_score":0.033269234,"about_ca_system_score_codex":0.00066677824,"about_ca_system_score_gemma":0.00065645005,"threshold_uncertainty_score":0.06615114},"labels":[],"label_agreement":null},{"id":"W1994058135","doi":"10.1086/527541","title":"Abundance Anomalies in Horizontal Branch Stars and Atomic Diffusion","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Horizontal branch; Stars; Astrophysics; Diffusion; Abundance (ecology); Astronomy; Globular cluster","score_opus":0.008128578611701933,"score_gpt":0.20502595053124695,"score_spread":0.196897371919545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994058135","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99558854,0.0005226903,0.0005970648,0.0005968684,0.000022764796,0.0000016634419,0.00021772791,0.00003081954,0.0024218766],"genre_scores_gemma":[0.99851316,0.00025744954,0.00017119393,0.000020098365,0.000044842927,7.794059e-7,0.00012856141,0.000010046121,0.00085378473],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999609,0.000004583245,0.0000032239468,0.000015875756,0.000008389825,0.000007067649],"domain_scores_gemma":[0.9993414,0.00022309985,0.00016230751,0.00003438123,0.00012408994,0.00011465647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032688706,0.00011823435,0.00022735143,0.0007539467,0.0003599071,0.00078584714,0.00020680268,0.00039607668,0.0022186951],"category_scores_gemma":[0.0021236057,0.00013957763,0.00012056292,0.00094072823,0.00030673193,0.0007941933,0.00046999977,0.00035252614,0.00019598259],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003005576,0.000038604376,0.9259315,0.00004344726,0.000073338335,0.00021228501,0.00034423592,0.0025055916,0.037703276,0.009130256,0.001299207,0.022417655],"study_design_scores_gemma":[0.00001090927,0.000024351006,0.9829222,0.0000067161363,0.00002207018,0.00018757902,0.000286187,0.005170234,0.002951129,0.0063896277,0.0020182517,0.000010888035],"about_ca_topic_score_codex":0.0025496436,"about_ca_topic_score_gemma":0.0031206876,"teacher_disagreement_score":0.0025496436,"about_ca_system_score_codex":0.0004016707,"about_ca_system_score_gemma":0.00015031178,"threshold_uncertainty_score":0.0074222684},"labels":[],"label_agreement":null},{"id":"W1994124960","doi":"10.1088/0004-637x/761/2/140","title":"A REDSHIFT SURVEY OF<i>HERSCHEL</i>FAR-INFRARED SELECTED STARBURSTS AND IMPLICATIONS FOR OBSCURED STAR FORMATION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":172,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of British Columbia","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Centre National d’Etudes Spatiales; Key Programme; Science and Technology Facilities Council; Centre National de la Recherche Scientifique; National Science Foundation; Imperial College London; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Space Telescope Science Institute; UK Space Agency","keywords":"Physics; Astrophysics; Redshift; Galaxy; Spire (mollusc); Luminous infrared galaxy; Astronomy; Infrared; Luminosity; Star formation; Spectral energy distribution","score_opus":0.016367404217974196,"score_gpt":0.24161054581978475,"score_spread":0.22524314160181055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994124960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99549025,0.0001985096,0.0001239614,0.00004977562,0.0000011746429,0.0000070368496,0.0030387323,0.000023240225,0.0010673361],"genre_scores_gemma":[0.99270296,0.00020500402,0.0005001494,0.000036661306,0.0000065966096,0.0000075578732,0.00584597,0.000008514418,0.0006866029],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967265,0.000053186766,0.00002406354,0.00009543163,0.0000868513,0.00006776144],"domain_scores_gemma":[0.99828786,0.0001539877,0.0009769901,0.0001449645,0.00017600192,0.0002601549],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053836906,0.00018905848,0.00013124199,0.002348556,0.0002745764,0.0004670328,0.00032163734,0.000194495,0.0014855313],"category_scores_gemma":[0.00084445975,0.00012274619,0.00013806754,0.001682845,0.00026454288,0.0005095998,0.00051580643,0.00017251974,0.00049766584],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030454705,0.000016369744,0.99369437,0.000016396009,0.000023810753,0.000043612916,0.00016375203,0.0001318441,0.0016922744,0.00011210507,0.00039947848,0.0036755663],"study_design_scores_gemma":[0.0000013179015,0.0000074034015,0.99924785,0.0000021032067,0.0000031902848,0.000044710392,0.000044606175,0.00007814373,0.00014804558,0.00001117619,0.0004101651,0.0000013237085],"about_ca_topic_score_codex":0.01830242,"about_ca_topic_score_gemma":0.0451036,"teacher_disagreement_score":0.01830242,"about_ca_system_score_codex":0.00075558596,"about_ca_system_score_gemma":0.00031262776,"threshold_uncertainty_score":0.036391735},"labels":[],"label_agreement":null},{"id":"W1994185228","doi":"10.1086/376895","title":"Three Lynds Bright Nebulae","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Young stellar object; Ionization; Reflection nebula; Astronomy; Galactic plane; Plasma; Stars; Planetary nebula; Star formation; Ion","score_opus":0.01073017166488646,"score_gpt":0.21581462114687333,"score_spread":0.20508444948198687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994185228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879411,0.00031884035,0.00027001963,0.00006299012,0.000008889703,0.00003466567,0.0006451332,0.000034654364,0.0106836455],"genre_scores_gemma":[0.9915998,0.0001586902,0.000797515,0.00008533169,0.0000072330636,0.000018986111,0.0016385604,0.000012523516,0.0056814086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996941,0.0000096753165,0.000015239841,0.00008041642,0.0000923112,0.00010825279],"domain_scores_gemma":[0.99970406,0.00002248286,0.00004241919,0.00001815135,0.00003942912,0.00017341369],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021832115,0.0002268045,0.00035655944,0.0015500963,0.0021649553,0.0009368971,0.00049204065,0.00029235875,0.002959633],"category_scores_gemma":[0.0004420931,0.00019698545,0.00023897536,0.00074526476,0.00079976884,0.00029185493,0.0015658127,0.00029045617,0.00037221503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005531353,0.00008702293,0.87661487,0.00015549609,0.000057959365,0.0025180883,0.005543195,0.00029736318,0.06759964,0.0023884838,0.0019632203,0.04222147],"study_design_scores_gemma":[0.000026616386,0.0000796931,0.97793293,0.000016826558,0.000023344215,0.0017246663,0.0019900622,0.00016536353,0.0038887458,0.00024082311,0.0138870645,0.000023745031],"about_ca_topic_score_codex":0.17308423,"about_ca_topic_score_gemma":0.339911,"teacher_disagreement_score":0.17308423,"about_ca_system_score_codex":0.002495213,"about_ca_system_score_gemma":0.0009697487,"threshold_uncertainty_score":0.34415352},"labels":[],"label_agreement":null},{"id":"W1994189809","doi":"10.1088/0004-637x/791/1/66","title":"SEEING RED IN M32: CONSTRAINTS ON THE STELLAR CONTENT FROM NEAR- AND MID-INFRARED OBSERVATIONS AND APPLICATIONS FOR STUDIES OF MORE DISTANT GALAXIES<sup>,</sup><sup>,</sup>","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Asymptotic giant branch; Stars; Galaxy; Infrared; Globular cluster; Elliptical galaxy; Astronomy; Luminosity","score_opus":0.03004657834270661,"score_gpt":0.23992685824354856,"score_spread":0.20988027990084196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994189809","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99436104,0.00086604967,0.0027018294,0.00021303348,0.0000050751705,0.000008857529,0.00033655207,0.00006865616,0.0014388672],"genre_scores_gemma":[0.99437594,0.0002316029,0.004641973,0.000036156824,0.000015202548,0.0000068857867,0.00045525882,0.000019496421,0.00021752142],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999007,0.000023293089,0.0000042721713,0.00003730655,0.000018838615,0.000015601014],"domain_scores_gemma":[0.9994537,0.000096454605,0.00019088034,0.000095983414,0.00005601536,0.000106937725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072149234,0.00040665586,0.00029319135,0.0006262178,0.00034725328,0.00063860806,0.0005838113,0.0006682567,0.0013660587],"category_scores_gemma":[0.0013531568,0.00024888915,0.00037935184,0.0008301779,0.0002887132,0.001038043,0.0009013295,0.0003403701,0.0007157981],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002641092,0.00003450375,0.9170955,0.00013001429,0.000052462332,0.00020893435,0.00060488016,0.0034440963,0.039838284,0.0012453092,0.0006237589,0.03645818],"study_design_scores_gemma":[0.000010644808,0.00007454659,0.9776993,0.000048586728,0.000041702744,0.0002493846,0.00040139214,0.015373214,0.002265638,0.0017064316,0.0021085036,0.000020634967],"about_ca_topic_score_codex":0.0042213746,"about_ca_topic_score_gemma":0.009632187,"teacher_disagreement_score":0.0042213746,"about_ca_system_score_codex":0.0005076818,"about_ca_system_score_gemma":0.00020170627,"threshold_uncertainty_score":0.008393645},"labels":[],"label_agreement":null},{"id":"W1994210724","doi":"10.1088/0004-637x/797/2/74","title":"TESTING MAGNETIC FIELD MODELS FOR THE CLASS 0 PROTOSTAR L1527","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Polarization (electrochemistry); Magnetic field; Polarimetry; Stokes parameters; Molecular cloud; Core (optical fiber); Field (mathematics)","score_opus":0.020347928221529223,"score_gpt":0.24274775067297538,"score_spread":0.22239982245144616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994210724","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991315,0.000013451508,0.00024245375,0.000015991238,0.0000017529899,0.0000074916125,0.000084441315,0.000012601465,0.0004902102],"genre_scores_gemma":[0.999432,0.000014711228,0.00018095542,0.000011274704,0.0000020355144,0.0000057827315,0.0002774831,0.000007088908,0.0000686333],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997688,0.000059455735,0.000012511794,0.000066683984,0.00004370961,0.00004879579],"domain_scores_gemma":[0.99912125,0.00031442713,0.000144505,0.000089103734,0.00009879971,0.00023191389],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066735735,0.00044036127,0.0003054893,0.0006965688,0.000473113,0.0008528027,0.00076897925,0.00046505302,0.0007083913],"category_scores_gemma":[0.001244586,0.00020887532,0.0005759013,0.00031160322,0.00056225824,0.00034833816,0.00053875736,0.00021204523,0.00022763078],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011777333,0.00034056292,0.7536944,0.000092698465,0.00031574335,0.00037828996,0.0005392683,0.20714048,0.02442164,0.0031799742,0.00074100203,0.007978284],"study_design_scores_gemma":[0.0003847474,0.0012727857,0.453079,0.0000318966,0.00012832064,0.00019215357,0.0014093313,0.5321161,0.0077095837,0.0022185682,0.001376209,0.000081340055],"about_ca_topic_score_codex":0.02574102,"about_ca_topic_score_gemma":0.012438789,"teacher_disagreement_score":0.02574102,"about_ca_system_score_codex":0.001780972,"about_ca_system_score_gemma":0.0008071947,"threshold_uncertainty_score":0.05118239},"labels":[],"label_agreement":null},{"id":"W1994290663","doi":"10.1088/0004-637x/693/2/1736","title":"THE JAMES CLERK MAXWELL TELESCOPE NEARBY GALAXIES LEGACY SURVEY. I. STAR-FORMING MOLECULAR GAS IN VIRGO CLUSTER SPIRAL GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; National Research Council Canada; McMaster University; Queen's University; Royal Military College of Canada; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Virgo Cluster; Astrophysics; Galaxy; Spiral galaxy; James Clerk Maxwell Telescope; Star formation; Luminosity; Interstellar medium; Astronomy; Hubble sequence; Line (geometry); Telescope; Cluster (spacecraft); Galaxy cluster; Geometry","score_opus":0.00783009507390548,"score_gpt":0.21942118839874045,"score_spread":0.21159109332483497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994290663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8594593,0.0021327292,0.0006488148,0.00046118555,0.00004864245,0.00010183967,0.11439675,0.00032674678,0.02242393],"genre_scores_gemma":[0.86864275,0.0018288766,0.002647138,0.00039280922,0.00010819704,0.00009857871,0.10885555,0.00008895438,0.017337168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981266,0.00001550756,0.000013867795,0.0000581562,0.000044848817,0.000055077835],"domain_scores_gemma":[0.9992111,0.000024972673,0.00026801517,0.00008154271,0.00009250677,0.00032176456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034443446,0.0002405426,0.00022418324,0.0035725757,0.0006294877,0.0006166441,0.0004455088,0.00022705484,0.0060702534],"category_scores_gemma":[0.0005602366,0.00017269567,0.00018719584,0.003215243,0.00019775609,0.000429812,0.00083533936,0.00022189888,0.002351694],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001162544,0.000050893243,0.9549568,0.00009290724,0.00008702869,0.00010072991,0.00048578586,0.000120568955,0.003011177,0.0006432322,0.021644507,0.018690174],"study_design_scores_gemma":[0.0000052433275,0.000010361345,0.9882025,0.000008492817,0.000011997175,0.00004453323,0.00008086098,0.00004175379,0.000081752834,0.000035243906,0.011474569,0.0000027012995],"about_ca_topic_score_codex":0.10230865,"about_ca_topic_score_gemma":0.18473092,"teacher_disagreement_score":0.10230865,"about_ca_system_score_codex":0.0009841964,"about_ca_system_score_gemma":0.00052808714,"threshold_uncertainty_score":0.2034263},"labels":[],"label_agreement":null},{"id":"W1994353135","doi":"10.1086/312483","title":"The Dwarf Irregular Galaxy UGC 7636 Exposed: Stripping at Work in the Virgo Cluster","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Virgo Cluster; Astrophysics; Physics; Dwarf galaxy; Galaxy; Irregular galaxy; Astronomy; Luminosity; Galaxy cluster; Interacting galaxy","score_opus":0.007662795033502204,"score_gpt":0.20275416523404272,"score_spread":0.19509137020054051,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994353135","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99975926,0.000019929976,0.0000061099095,0.0000078807325,3.9670087e-7,8.5203686e-7,0.000046320733,0.0000020404498,0.00015723844],"genre_scores_gemma":[0.9996431,0.000017999364,0.000039485036,0.0000063898324,0.0000011368595,5.2603724e-7,0.000117592775,0.0000011109637,0.00017264573],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987316,0.0000089369705,0.0000037361149,0.000026848462,0.000020969232,0.000066345274],"domain_scores_gemma":[0.9997036,0.000020171608,0.00006783091,0.000037114434,0.000018636378,0.00015270487],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009481349,0.00023756346,0.00027031082,0.00088706805,0.0009851294,0.0003906186,0.0002620961,0.0002792285,0.00082919403],"category_scores_gemma":[0.00036128925,0.00012711599,0.00014793662,0.0009982621,0.0006856423,0.00020875188,0.0008572821,0.00025639433,0.00022335716],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091452844,0.00015805154,0.95320976,0.000028883993,0.000050815346,0.0015798991,0.0022097488,0.0007807895,0.030697195,0.00045980644,0.0004945262,0.009416041],"study_design_scores_gemma":[0.0000057847983,0.00005369623,0.9974312,0.0000019668369,0.000012193555,0.0003312898,0.00051321567,0.00020613278,0.0009025918,0.00009609789,0.00043951382,0.0000064134188],"about_ca_topic_score_codex":0.07695605,"about_ca_topic_score_gemma":0.07031954,"teacher_disagreement_score":0.07695605,"about_ca_system_score_codex":0.0010016551,"about_ca_system_score_gemma":0.0002715942,"threshold_uncertainty_score":0.15301621},"labels":[],"label_agreement":null},{"id":"W1994462522","doi":"10.1088/0004-637x/743/2/102","title":"HIGH-PRECISION TIMING OF FIVE MILLISECOND PULSARS: SPACE VELOCITIES, BINARY EVOLUTION, AND EQUIVALENCE PRINCIPLES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Swinburne University of Technology; Commonwealth Scientific and Industrial Research Organisation; National Science Foundation","keywords":"Pulsar; Physics; Millisecond pulsar; Binary number; Astrophysics; Binary pulsar; Parameter space; Proper motion; Range (aeronautics); Binary system; Statistics; Mathematics; Stars","score_opus":0.03099795732508846,"score_gpt":0.29264260347558135,"score_spread":0.2616446461504929,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994462522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98702,0.0005579436,0.010864552,0.00002878449,0.000017290611,0.0000118874705,0.00024421103,0.00008938351,0.0011658581],"genre_scores_gemma":[0.9919876,0.00006987229,0.0074802553,0.0000068266027,0.000016574515,0.0000056333683,0.00030464318,0.000013222071,0.00011547314],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99961805,0.00005268731,0.00002592296,0.00013645356,0.00013080228,0.000036012196],"domain_scores_gemma":[0.9987587,0.0002628797,0.00046219863,0.00019339017,0.00022835487,0.00009456452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00086034136,0.00020170282,0.00027772787,0.0009996516,0.00036269138,0.000618793,0.0003489823,0.00024852494,0.00034238174],"category_scores_gemma":[0.0021475141,0.0001547275,0.0001593957,0.0009836209,0.00028623067,0.00048086207,0.00061833754,0.0004315227,0.000097299504],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005903014,0.00009790743,0.5415101,0.00020951357,0.00030824708,0.00044992773,0.001316556,0.009196,0.27927968,0.0019841804,0.0004887414,0.16456884],"study_design_scores_gemma":[0.000034219258,0.00032749923,0.921968,0.000017850063,0.00012571004,0.0009176008,0.00013465309,0.018814206,0.053914603,0.00084409246,0.0028622334,0.000039403483],"about_ca_topic_score_codex":0.0016586912,"about_ca_topic_score_gemma":0.0027062986,"teacher_disagreement_score":0.0016586912,"about_ca_system_score_codex":0.00024981063,"about_ca_system_score_gemma":0.00013832859,"threshold_uncertainty_score":0.00455004},"labels":[],"label_agreement":null},{"id":"W1994531398","doi":"10.1086/508533","title":"The Mass of the Black Hole in the Seyfert 1 Galaxy NGC 4593 from Reverberation Mapping","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Ohio State University; CRDF Global; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Astrophysics; Reverberation mapping; Galaxy; Light curve; Black hole (networking); Observatory; Line (geometry); Reverberation; Emission spectrum; Supermassive black hole; Astronomy; Spectral line; Geometry","score_opus":0.006549305963883792,"score_gpt":0.1931986731901209,"score_spread":0.18664936722623712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994531398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989341,0.0001534154,0.00041730874,0.000011934353,0.0000028538618,0.00000176987,0.00012926363,0.00003526421,0.00031401735],"genre_scores_gemma":[0.99884784,0.00008841733,0.0006205666,0.000006485443,0.000010068367,0.0000021805647,0.00033232555,0.0000067024257,0.00008522975],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990356,0.000011282745,0.0000049252035,0.000036689093,0.000021230535,0.000022313689],"domain_scores_gemma":[0.9996532,0.00004675473,0.00013659676,0.000079119796,0.000032284814,0.00005208674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026826918,0.00048472753,0.00037083868,0.001016245,0.00022885423,0.0005410549,0.0003883607,0.00034319004,0.00086462224],"category_scores_gemma":[0.0007826843,0.00018031472,0.00032583103,0.00043261482,0.00026152848,0.00045767266,0.00048405875,0.00026955007,0.00036155523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006988141,0.000077737066,0.7921227,0.00008840171,0.00021812152,0.0018865471,0.0019199355,0.006517035,0.1318302,0.00072860543,0.0008165513,0.06309535],"study_design_scores_gemma":[0.000008376411,0.0000762631,0.98943245,0.000007975535,0.00006203152,0.0005489148,0.000110385874,0.0030149128,0.0056439713,0.00023687983,0.0008419222,0.000015874622],"about_ca_topic_score_codex":0.0047682794,"about_ca_topic_score_gemma":0.006185165,"teacher_disagreement_score":0.0047682794,"about_ca_system_score_codex":0.00039914993,"about_ca_system_score_gemma":0.000060792056,"threshold_uncertainty_score":0.009481072},"labels":[],"label_agreement":null},{"id":"W1994573710","doi":"10.1088/0004-637x/763/2/72","title":"THE HELICAL JET OF THE VELA PULSAR","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Vela; Pulsar; Physics; Nebula; Astrophysics; Neutron star; Astronomy; Precession; Jet (fluid); Sky; Proper motion; Observatory; Stars","score_opus":0.008701202536899636,"score_gpt":0.28921544656171916,"score_spread":0.2805142440248195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994573710","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988758,0.00007764701,0.00023992536,0.000017002038,0.000004372677,0.0000014294906,0.000072186784,0.000009598067,0.00070210575],"genre_scores_gemma":[0.9993338,0.000049509777,0.00025101687,0.000007300505,0.000007626984,0.0000020648379,0.00016512405,0.0000038004125,0.00017975057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999579,0.0000073351807,0.000001972216,0.000012289905,0.0000072834446,0.000013151261],"domain_scores_gemma":[0.9997949,0.000048337042,0.00007117258,0.000027312752,0.000017251516,0.00004108631],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011538613,0.00008142275,0.00014301596,0.0003595772,0.0002994276,0.0005044458,0.00011020805,0.00011110283,0.00041885758],"category_scores_gemma":[0.0005419039,0.000098680444,0.00008303044,0.00033162054,0.00023943241,0.00021456386,0.00031714668,0.000183221,0.0000886425],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010716122,0.00013226013,0.6642409,0.00009803613,0.00016357792,0.0059473375,0.0016780966,0.026473045,0.25986853,0.0074359165,0.0013230185,0.03156778],"study_design_scores_gemma":[0.00003800289,0.00021173035,0.9628694,0.000024260227,0.00003920399,0.0013660728,0.00053519936,0.02013364,0.009146294,0.002082907,0.003518484,0.000034819703],"about_ca_topic_score_codex":0.001105919,"about_ca_topic_score_gemma":0.00096379564,"teacher_disagreement_score":0.001105919,"about_ca_system_score_codex":0.00014250114,"about_ca_system_score_gemma":0.00010672664,"threshold_uncertainty_score":0.0021989346},"labels":[],"label_agreement":null},{"id":"W1994619117","doi":"10.1086/499558","title":"Connecting Galaxy Evolution, Star Formation, and the Cosmic X‐Ray Background","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy; X-ray background; Star formation; Galaxy formation and evolution; COSMIC cancer database; Cosmic ray; Star (game theory); Active galactic nucleus","score_opus":0.00704586034031126,"score_gpt":0.20304286875805155,"score_spread":0.1959970084177403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994619117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952697,0.0002010701,0.0020614923,0.000056969588,0.000004298328,0.0000059896115,0.00016197181,0.00006882108,0.0021697986],"genre_scores_gemma":[0.9986357,0.000089774185,0.0006292813,0.000013159048,0.000002167156,0.000003084318,0.00015685949,0.000012399172,0.00045745925],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99989164,0.000037072026,0.0000041405233,0.000026948592,0.000010385446,0.000029728782],"domain_scores_gemma":[0.99958605,0.00019582403,0.00008847617,0.000041745425,0.000033023884,0.00005493574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034769485,0.00042897058,0.00023161442,0.00043693063,0.00030108102,0.0015743731,0.0004389491,0.00045524514,0.0019842687],"category_scores_gemma":[0.0014645527,0.0002734264,0.00038169543,0.00049088756,0.00047113595,0.00063470803,0.0003970496,0.00032321486,0.0002849102],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012887736,0.00006169949,0.43293878,0.000036251822,0.00013569207,0.000161052,0.00013599108,0.54506767,0.0030497706,0.010154844,0.00032182733,0.0078074164],"study_design_scores_gemma":[0.000035930756,0.00013674588,0.1587144,0.000014624934,0.00007505156,0.0002126243,0.00014375139,0.82926506,0.001480649,0.008132771,0.0017638247,0.000024577113],"about_ca_topic_score_codex":0.022030368,"about_ca_topic_score_gemma":0.015215755,"teacher_disagreement_score":0.022030368,"about_ca_system_score_codex":0.0012249816,"about_ca_system_score_gemma":0.0003975438,"threshold_uncertainty_score":0.04380423},"labels":[],"label_agreement":null},{"id":"W1994700211","doi":"10.1086/308457","title":"Space Telescope Imaging Spectrograph Long‐Slit Spectroscopy of the Narrow‐Line Region of NGC 4151. II. Physical Conditions along Position Angle 221o","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Space Telescope Imaging Spectrograph; Astrophysics; Galaxy; Photoionization; Spectral line; Astronomy; Ionization; Telescope; Position angle; Line (geometry); Spectrograph; Doubly ionized oxygen; Line-of-sight; Emission spectrum; Hubble space telescope; Geometry","score_opus":0.004614294037363301,"score_gpt":0.21786531794919758,"score_spread":0.2132510239118343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994700211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99654937,0.00007190446,0.0004101647,0.00003145833,0.000002889675,0.000010531616,0.0011762113,0.00007842686,0.001668998],"genre_scores_gemma":[0.9950016,0.000063791325,0.0013185154,0.000024295143,0.0000063789457,0.0000116043075,0.002549724,0.000013440194,0.001010606],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992824,0.0000087104845,0.000004853175,0.000022913948,0.000019643048,0.000015544],"domain_scores_gemma":[0.9997098,0.00003387256,0.00010226794,0.000035827223,0.00004899743,0.000069291724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020681137,0.00020106531,0.00011042485,0.0007240222,0.00047595298,0.00032650208,0.00017651795,0.00016719871,0.001635926],"category_scores_gemma":[0.00025761878,0.000126156,0.00012507365,0.00054571003,0.00011397916,0.00020338701,0.00022757544,0.00018013772,0.0002962168],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003939665,0.00019054137,0.84228545,0.000092242306,0.000092507995,0.0006533082,0.00091179047,0.003083772,0.13158321,0.0005491196,0.001766518,0.018397579],"study_design_scores_gemma":[0.000008635255,0.000046801608,0.9944377,0.000004004966,0.000017328162,0.00012285709,0.00010436345,0.0011976894,0.0029073644,0.000051406612,0.0010975088,0.0000044483813],"about_ca_topic_score_codex":0.008599592,"about_ca_topic_score_gemma":0.02383053,"teacher_disagreement_score":0.008599592,"about_ca_system_score_codex":0.00036834358,"about_ca_system_score_gemma":0.00015357864,"threshold_uncertainty_score":0.017099023},"labels":[],"label_agreement":null},{"id":"W1994711528","doi":"10.1086/338221","title":"Constraints on the Size Evolution of Brightest Cluster Galaxies","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Redshift; Physics; Galaxy; Surface brightness; Astronomy; Luminosity; Cluster (spacecraft); Accretion (finance); Galaxy cluster; RADIUS; Star formation","score_opus":0.00891632101834837,"score_gpt":0.19655084915923587,"score_spread":0.1876345281408875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994711528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980719,0.00008793868,0.00037607786,0.000031310323,0.0000014904717,0.0000024615756,0.00019993336,0.000024926225,0.0012039371],"genre_scores_gemma":[0.99899703,0.000023670438,0.00036287337,0.000012018886,0.0000047393414,0.0000026264017,0.0004254124,0.0000071472573,0.00016445151],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962974,0.000047948844,0.00001619162,0.000122037025,0.00006591728,0.000118153366],"domain_scores_gemma":[0.9965649,0.00080423563,0.0010358242,0.0004657292,0.00040378293,0.00072554295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074556883,0.0002492147,0.00022621533,0.0013653412,0.00051505945,0.000988847,0.0006407025,0.00034625063,0.0011691455],"category_scores_gemma":[0.0036999474,0.00032223124,0.0002026043,0.00051035883,0.00047113103,0.00052016217,0.00081267674,0.000248808,0.00036176504],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007839114,0.000016784661,0.98905456,0.000006752793,0.000016071606,0.00002910983,0.00013819852,0.0005757671,0.0057832,0.00035515052,0.00019392946,0.0037520586],"study_design_scores_gemma":[0.0000037899722,0.000014729454,0.9966426,0.0000034801533,0.0000086749105,0.00005249743,0.00007517371,0.0016995709,0.0010415419,0.000146456,0.0003063952,0.00000508344],"about_ca_topic_score_codex":0.015255073,"about_ca_topic_score_gemma":0.025239298,"teacher_disagreement_score":0.015255073,"about_ca_system_score_codex":0.0006141845,"about_ca_system_score_gemma":0.00024145348,"threshold_uncertainty_score":0.030332565},"labels":[],"label_agreement":null},{"id":"W1994729568","doi":"10.1088/0004-637x/700/2/1034","title":"MULTIWAVELENGTH OBSERVATIONS OF LS I +61° 303 WITH VERITAS,<i>SWIFT</i>, AND<i>RXTE</i>","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Swift; Flux (metallurgy); Orbital period; Binary number; Astronomy; Stars","score_opus":0.010056852266510168,"score_gpt":0.20820736473200163,"score_spread":0.19815051246549145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994729568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963858,0.00007721597,0.00013677093,0.000018571127,0.0000049796095,0.000009235149,0.0012399865,0.000025428812,0.0021019697],"genre_scores_gemma":[0.9929183,0.00007375744,0.00089684495,0.000042415242,0.000015743648,0.000011476479,0.0050684917,0.000013961073,0.00095900224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997979,0.000016326447,0.000009240071,0.000051400722,0.00007092792,0.000054151507],"domain_scores_gemma":[0.9994598,0.000041918425,0.000256478,0.000049683276,0.000070521026,0.0001214933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000231087,0.00017257848,0.00022695202,0.00065661996,0.00048891694,0.00039050725,0.00023417466,0.00027906802,0.0017136373],"category_scores_gemma":[0.00027465727,0.00016029862,0.00014329333,0.00079226313,0.0002298913,0.0002148697,0.00046228088,0.0003333522,0.0005729139],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056651543,0.0002129508,0.9159199,0.00006676625,0.00006967019,0.00044090886,0.00050787296,0.00079787057,0.05769654,0.00027280548,0.0023868654,0.021061348],"study_design_scores_gemma":[0.00000808431,0.0001021653,0.9969175,0.0000043091864,0.000008067736,0.00017302038,0.00007604614,0.00021353291,0.00084641576,0.000019134952,0.0016277899,0.000003977551],"about_ca_topic_score_codex":0.013984797,"about_ca_topic_score_gemma":0.066781454,"teacher_disagreement_score":0.013984797,"about_ca_system_score_codex":0.00053779385,"about_ca_system_score_gemma":0.00030228787,"threshold_uncertainty_score":0.027806818},"labels":[],"label_agreement":null},{"id":"W1994821169","doi":"10.1088/0004-637x/789/2/119","title":"A 1.05<i>M</i><sub>☉</sub>COMPANION TO PSR J2222–0137: THE COOLEST KNOWN WHITE DWARF?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"White dwarf; Physics; Astrophysics; Neutron star; Pulsar; Astronomy; Low Mass; Stars","score_opus":0.009247740289023436,"score_gpt":0.2797262466369543,"score_spread":0.27047850634793086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994821169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99328977,0.00016344403,0.000302151,0.00022869212,0.00002877644,0.000007439072,0.00016525196,0.00009037262,0.005724115],"genre_scores_gemma":[0.99812526,0.000027604081,0.0003596327,0.00006452183,0.000014574573,0.0000014857828,0.00019933403,0.000009869553,0.0011977564],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999335,0.0000042045676,0.000003979066,0.000022187272,0.000017339073,0.000018905828],"domain_scores_gemma":[0.9998141,0.000011957506,0.000052982712,0.00001672529,0.000020593658,0.00008356905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000117631585,0.00019466515,0.00021844005,0.00027310493,0.00055021973,0.0005503469,0.000358626,0.00037762983,0.0032815882],"category_scores_gemma":[0.0003825172,0.0001143772,0.000096179705,0.00022713258,0.0003361087,0.00034647188,0.00037382788,0.00022155112,0.0011162929],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006412248,0.00019999902,0.8231038,0.000092089744,0.00007508394,0.0077906186,0.0010724177,0.0006061166,0.11542984,0.0057771388,0.008635238,0.03657647],"study_design_scores_gemma":[0.00004449472,0.0006589727,0.9136485,0.000022204618,0.000102543556,0.014524095,0.0016667439,0.005479248,0.030331612,0.002285063,0.03119854,0.000037951973],"about_ca_topic_score_codex":0.008221948,"about_ca_topic_score_gemma":0.009850656,"teacher_disagreement_score":0.008221948,"about_ca_system_score_codex":0.0005967339,"about_ca_system_score_gemma":0.00026655334,"threshold_uncertainty_score":0.016348183},"labels":[],"label_agreement":null},{"id":"W1994826799","doi":"10.1086/507019","title":"High‐Mass Star Formation. III. The Functional Form of the Submillimeter Clump Mass Function","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Mass distribution; Power law; Physics; Initial mass function; Star formation; Log-normal distribution; Fragmentation (computing); Exponent; Stars; Statistics; Galaxy; Mathematics; Biology","score_opus":0.007999255831321387,"score_gpt":0.19071480727841886,"score_spread":0.18271555144709747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994826799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99253005,0.00023281129,0.0046864194,0.000062989,0.0000051033862,0.0000133332,0.00031519978,0.000098350225,0.0020557332],"genre_scores_gemma":[0.99857914,0.000024444593,0.0008927291,0.0000144717305,0.0000032578275,0.0000060635443,0.00023272967,0.000016015323,0.00023126412],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998198,0.000030523763,0.000009994034,0.0000541019,0.00003978958,0.000045713434],"domain_scores_gemma":[0.9983367,0.0006444933,0.0005097181,0.00019982092,0.00016518471,0.00014413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00083113846,0.00038622538,0.00027829935,0.0010423493,0.00024543545,0.00075433234,0.0005609508,0.0005329319,0.0013459385],"category_scores_gemma":[0.0030511648,0.00024634838,0.00054489396,0.00060478196,0.00041579787,0.0004720841,0.000447894,0.00033131274,0.0006695923],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013487657,0.000029700646,0.95093584,0.00006093061,0.00009316646,0.00025125936,0.00018515557,0.01452092,0.016779436,0.0018516794,0.00041282503,0.014744274],"study_design_scores_gemma":[0.000012108325,0.0000506779,0.95317876,0.000012763547,0.000020560332,0.00042753856,0.000107066284,0.04123288,0.0030402087,0.0012089973,0.0006971007,0.0000113507695],"about_ca_topic_score_codex":0.0017711594,"about_ca_topic_score_gemma":0.001363687,"teacher_disagreement_score":0.0017711594,"about_ca_system_score_codex":0.00053125416,"about_ca_system_score_gemma":0.00012908969,"threshold_uncertainty_score":0.0045025945},"labels":[],"label_agreement":null},{"id":"W1994827287","doi":"10.1086/521600","title":"On the Use of Blanketed Atmospheres as Boundary Conditions for Stellar Evolutionary Models","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Hydrostatic equilibrium; Photosphere; Stars; Atmosphere (unit); Stellar atmosphere; Open cluster; Effective temperature; Astronomy; Thermodynamics; Spectral line","score_opus":0.03826233577764085,"score_gpt":0.24133969975446584,"score_spread":0.203077363976825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994827287","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3323491,0.0007356718,0.6411412,0.00051114004,0.00013281191,0.0001892234,0.000897718,0.0019206296,0.022122512],"genre_scores_gemma":[0.88916034,0.0002800866,0.10625737,0.00010413136,0.00007322917,0.00019381005,0.0005768539,0.0007163662,0.0026378494],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993068,0.00036827018,0.000036629033,0.00008729949,0.00013817035,0.000062845174],"domain_scores_gemma":[0.99720806,0.0015787971,0.00023163632,0.00048554514,0.00030487304,0.0001910239],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022078499,0.00079325464,0.00077710714,0.00075357466,0.0011023759,0.00193873,0.002342643,0.0009974517,0.0025065716],"category_scores_gemma":[0.011292912,0.0005982658,0.0010575942,0.00046282675,0.00096674875,0.0021709711,0.0019008848,0.0015315878,0.0008048168],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000120453,0.00004287346,0.0053508175,0.000039917817,0.000050872528,0.00012401493,0.00019412403,0.9307906,0.0013648078,0.05288374,0.00040707667,0.008630656],"study_design_scores_gemma":[0.000022230495,0.00002080333,0.0005763815,0.000021242146,0.000011943671,0.000023990979,0.000021965405,0.9885533,0.00035846664,0.00942206,0.00095286744,0.000014824373],"about_ca_topic_score_codex":0.0065909177,"about_ca_topic_score_gemma":0.006773077,"teacher_disagreement_score":0.0065909177,"about_ca_system_score_codex":0.0010756601,"about_ca_system_score_gemma":0.0008187957,"threshold_uncertainty_score":0.013105094},"labels":[],"label_agreement":null},{"id":"W1994956090","doi":"10.1088/0004-637x/731/2/124","title":"DENSITY VARIATIONS IN THE NW STAR STREAM OF M31","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Andromeda; Andromeda Galaxy; Star (game theory); Luminosity; Star formation; Milky Way; Star cluster","score_opus":0.012658321101869685,"score_gpt":0.20706345093715942,"score_spread":0.19440512983528974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994956090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99971145,0.000009792355,0.000041298896,0.0000050454005,4.6685355e-7,9.589194e-7,0.000067172055,0.0000057282446,0.00015805387],"genre_scores_gemma":[0.99962306,0.000007694676,0.0000721605,0.0000021072858,9.702278e-7,9.944303e-7,0.00021217346,0.000001833113,0.00007904968],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989533,0.000016454156,0.0000058163973,0.00003412988,0.000023098632,0.000025108215],"domain_scores_gemma":[0.99939036,0.00019171489,0.00013003415,0.000067867884,0.00010423835,0.00011582696],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018217805,0.00009963383,0.00015709152,0.00038406116,0.00020860723,0.00036476718,0.00017313326,0.0002125537,0.0007313772],"category_scores_gemma":[0.0014099409,0.00009004069,0.00014511179,0.00042202545,0.00023241832,0.00017979933,0.00031540985,0.00011575885,0.00017253192],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027702827,0.0000846069,0.9578884,0.00001775735,0.000057919064,0.00037598025,0.00034417066,0.012821544,0.019433204,0.0006339771,0.0005103395,0.007555108],"study_design_scores_gemma":[0.000009339232,0.00007857506,0.97296077,0.0000029526364,0.0000134587435,0.00015125344,0.00013791154,0.024038088,0.002183993,0.000110948175,0.0003019473,0.000010845939],"about_ca_topic_score_codex":0.0052382206,"about_ca_topic_score_gemma":0.004549136,"teacher_disagreement_score":0.0052382206,"about_ca_system_score_codex":0.00035893606,"about_ca_system_score_gemma":0.00014032549,"threshold_uncertainty_score":0.010415494},"labels":[],"label_agreement":null},{"id":"W1994966998","doi":"10.1088/0004-637x/726/1/43","title":"MULTI-WAVELENGTH OBSERVATIONS OF THE FLARING GAMMA-RAY BLAZAR 3C 66A IN 2008 OCTOBER","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Blazar; Fermi Gamma-ray Space Telescope; BL Lac object; Astrophysics; Gamma ray; Spectral energy distribution; Compton scattering; Telescope; Wavelength; Light curve; Scattering; Radiation; Astronomy; Galaxy; Nuclear physics; Optics","score_opus":0.016434756544587904,"score_gpt":0.22610185017908926,"score_spread":0.20966709363450137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994966998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997405,0.00008846028,0.00019844693,0.000040587758,0.000007492173,0.000007675867,0.0010131267,0.00006262815,0.0011765332],"genre_scores_gemma":[0.9959869,0.00007351913,0.00077075645,0.000027062715,0.0000135998,0.0000045921283,0.0023581402,0.000012162297,0.000753196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992406,0.000004674481,0.0000033826148,0.000019217478,0.000023277045,0.000025479934],"domain_scores_gemma":[0.99982196,0.000010584899,0.00006672525,0.000019974725,0.000024824478,0.000055939836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017500596,0.00025513725,0.00023767243,0.00089211605,0.0004891563,0.0003929617,0.00016812803,0.00034148266,0.00066880905],"category_scores_gemma":[0.0002150066,0.00017587803,0.00022587676,0.0007260138,0.0001628814,0.00019810202,0.00033547854,0.00031508345,0.0002303984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023920753,0.00042963115,0.7134421,0.00017195812,0.00034167507,0.003615627,0.0015159969,0.0041808267,0.22498585,0.0008496692,0.004569339,0.043505263],"study_design_scores_gemma":[0.000020487983,0.000053091382,0.9940937,0.000006962513,0.000029055187,0.00026836584,0.00005363612,0.0009447847,0.002585256,0.000067609086,0.0018653445,0.0000115251505],"about_ca_topic_score_codex":0.014480336,"about_ca_topic_score_gemma":0.06455141,"teacher_disagreement_score":0.014480336,"about_ca_system_score_codex":0.00059643394,"about_ca_system_score_gemma":0.00017605771,"threshold_uncertainty_score":0.028792083},"labels":[],"label_agreement":null},{"id":"W1994987973","doi":"10.1088/0004-637x/754/1/21","title":"ROSSBY WAVE INSTABILITY IN LOCALLY ISOTHERMAL AND POLYTROPIC DISKS: THREE-DIMENSIONAL LINEAR CALCULATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Polytropic process; Physics; Instability; Hydrostatic equilibrium; Rossby number; Rossby wave; Vortex; Mechanics; Isothermal process; Classical mechanics; Turbulence; Thermodynamics; Quantum mechanics","score_opus":0.011592118061161404,"score_gpt":0.23627197448891366,"score_spread":0.22467985642775226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1994987973","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93117195,0.00037624445,0.042837203,0.00048064932,0.000049272396,0.00006232512,0.00067504635,0.0005775084,0.023769712],"genre_scores_gemma":[0.98206884,0.00017883356,0.014796889,0.00008828134,0.000022261345,0.000106882995,0.00023953729,0.00011812469,0.0023803446],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999081,0.000021980022,0.0000059392687,0.000009319894,0.000028568445,0.0000259784],"domain_scores_gemma":[0.99935335,0.00030808145,0.000104848135,0.00006092086,0.000099464,0.00007332064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026468717,0.0004262111,0.00065503333,0.0004371323,0.0007057956,0.00085732294,0.0009871493,0.00088380853,0.002562267],"category_scores_gemma":[0.0012669028,0.00028354226,0.00048312644,0.00057498866,0.0006631972,0.0004837006,0.0007363317,0.0006470966,0.00036990372],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008935883,0.000054385575,0.002564867,0.00006805916,0.000019012896,0.00022229928,0.00010605877,0.9835653,0.0035983406,0.0066614905,0.00039488016,0.002656064],"study_design_scores_gemma":[0.000020786436,0.000012357698,0.00050951797,0.000003571863,0.0000041082617,0.00001417751,0.000024297682,0.99793184,0.00037530067,0.00096587307,0.00013176995,0.0000063822044],"about_ca_topic_score_codex":0.011612042,"about_ca_topic_score_gemma":0.0070234053,"teacher_disagreement_score":0.011612042,"about_ca_system_score_codex":0.00096585846,"about_ca_system_score_gemma":0.0006705927,"threshold_uncertainty_score":0.023088872},"labels":[],"label_agreement":null},{"id":"W1995016890","doi":"10.1086/510771","title":"Molecular Cloud Evolution. II. From Cloud Formation to the Early Stages of Star Formation in Decaying Conditions","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":373,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Star formation; Molecular cloud; Physics; Gravitational collapse; Astrophysics; Stars; Turbulence; Velocity dispersion; Formation and evolution of the Solar System; Mechanics; Galaxy; Solar System","score_opus":0.009501639577074075,"score_gpt":0.2471449641908403,"score_spread":0.23764332461376625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995016890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960133,0.00009683528,0.0013055782,0.00007903058,0.0000052617984,0.000023278088,0.0001646374,0.000016909878,0.0022951958],"genre_scores_gemma":[0.99845684,0.00007285565,0.0007255729,0.000029646259,0.0000030016138,0.000013499219,0.00014129972,0.0000091839565,0.0005481272],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992573,0.000008606388,0.0000031265306,0.000011889656,0.00001108501,0.000039604944],"domain_scores_gemma":[0.9998171,0.000043022585,0.000045276534,0.000014125834,0.000024512292,0.00005595023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020664501,0.00021434118,0.00030343333,0.00028012175,0.00045172553,0.00071393483,0.00061658915,0.00068308366,0.0012893694],"category_scores_gemma":[0.0014111928,0.00018820936,0.00043528771,0.0003679935,0.0006858625,0.0007433358,0.0005675477,0.0006464842,0.00014017396],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004377531,0.0003531392,0.12770113,0.00014488127,0.00008610906,0.0011361135,0.0006162244,0.818844,0.021124283,0.019571813,0.0007006518,0.009283909],"study_design_scores_gemma":[0.00009225819,0.00024932384,0.039217457,0.000022478642,0.000028743547,0.0001645565,0.00029024476,0.95300704,0.0028884353,0.002733124,0.0012846845,0.000021581123],"about_ca_topic_score_codex":0.020395035,"about_ca_topic_score_gemma":0.010864373,"teacher_disagreement_score":0.020395035,"about_ca_system_score_codex":0.00090916426,"about_ca_system_score_gemma":0.0006513499,"threshold_uncertainty_score":0.040552676},"labels":[],"label_agreement":null},{"id":"W1995193687","doi":"10.1086/513067","title":"The Virgo Stellar Overdensity: Mapping the Infall of the Sagittarius Tidal Stream onto the Milky Way Disk","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Milky Way; Sagittarius; Astrophysics; Astronomy; Halo; Dark matter halo; Dark matter; Galaxy; Galactic plane","score_opus":0.011529593745394313,"score_gpt":0.2120446494612977,"score_spread":0.2005150557159034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995193687","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99922,0.0000403248,0.00022012574,0.000015412716,7.771363e-7,0.0000023246205,0.0000358369,0.000014022158,0.00045113076],"genre_scores_gemma":[0.99933225,0.000036411377,0.00042799025,0.000007424291,0.0000018286202,0.0000014325572,0.00008131101,0.000004930151,0.00010650848],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995553,0.000011312067,0.0000014458221,0.000010077052,0.000008526972,0.000013056057],"domain_scores_gemma":[0.99983585,0.000024910674,0.000039695686,0.00002077458,0.0000189972,0.000059793056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106417196,0.00011163585,0.00012465622,0.0005267921,0.0002620746,0.0003568992,0.00019535703,0.00017891977,0.0005625777],"category_scores_gemma":[0.00045831094,0.00014187772,0.00019523599,0.00040710578,0.00017344521,0.00021901124,0.000490443,0.00013630134,0.00012594156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030794382,0.00006636832,0.945305,0.00002551706,0.0000775527,0.00040403032,0.0007365535,0.003091172,0.033541307,0.00078691426,0.00040243482,0.015255262],"study_design_scores_gemma":[0.000009769729,0.00006013118,0.9853012,0.000008701609,0.00002714769,0.00023309988,0.00039611242,0.011077149,0.0016899821,0.00030735513,0.0008803829,0.000009172597],"about_ca_topic_score_codex":0.010873288,"about_ca_topic_score_gemma":0.019901743,"teacher_disagreement_score":0.010873288,"about_ca_system_score_codex":0.00034750643,"about_ca_system_score_gemma":0.00016942805,"threshold_uncertainty_score":0.021619976},"labels":[],"label_agreement":null},{"id":"W1995201090","doi":"10.1086/321682","title":"Long‐Term<i>Rossi X‐Ray Timing Explorer</i>Monitoring of the Anomalous X‐Ray Pulsar 1E 1048.1−5937","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Glitch; Physics; Astrophysics; Magnetar; X-ray pulsar; Neutron star; Astronomy; Flux (metallurgy); Precession; Static timing analysis","score_opus":0.02579365760842383,"score_gpt":0.3191409386456218,"score_spread":0.293347281037198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995201090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988707,0.000078646444,0.00018653563,0.000023217335,0.0000028616791,0.00000523981,0.00021247627,0.000015248415,0.000605017],"genre_scores_gemma":[0.99718386,0.00010300393,0.0010221049,0.000026880945,0.000012237917,0.000008744044,0.0012152009,0.000006844728,0.000421015],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999162,0.0000075464195,0.000005345174,0.000024004712,0.000022380656,0.00002449229],"domain_scores_gemma":[0.99971825,0.00002131411,0.00012653563,0.000030818734,0.00004770159,0.000055347475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019378457,0.00016569068,0.00016140153,0.00036247913,0.0002826179,0.00023641357,0.00018174377,0.00019930625,0.0002834039],"category_scores_gemma":[0.00034431362,0.000059303366,0.00009044756,0.00024694734,0.00016993834,0.00020889085,0.00029480897,0.00024759473,0.00013839403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035508384,0.0001468297,0.7311948,0.00006155526,0.000106628424,0.0013377351,0.00033008846,0.0007643965,0.22921175,0.00038827345,0.0010491485,0.035053723],"study_design_scores_gemma":[0.000010741701,0.00035982527,0.9833382,0.0000066215957,0.00004458808,0.0009999713,0.00007179258,0.00079219224,0.012181006,0.000112263995,0.0020698467,0.000013128301],"about_ca_topic_score_codex":0.0023576152,"about_ca_topic_score_gemma":0.0065021007,"teacher_disagreement_score":0.0023576152,"about_ca_system_score_codex":0.00016073667,"about_ca_system_score_gemma":0.00009572996,"threshold_uncertainty_score":0.004687786},"labels":[],"label_agreement":null},{"id":"W1995226241","doi":"10.1088/0004-637x/763/2/146","title":"THE OPACITY OF THE INTERGALACTIC MEDIUM DURING REIONIZATION: RESOLVING SMALL-SCALE STRUCTURE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; Physics; Opacity; Astrophysics; Structure formation; Redshift; Dark matter; Ionization; Adiabatic process; Universe; Mean free path; Galaxy; Scattering","score_opus":0.0044039682156389185,"score_gpt":0.18121709518300833,"score_spread":0.1768131269673694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995226241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99275887,0.00016170839,0.005722128,0.0001072857,0.0000069558364,0.000007600867,0.000090177484,0.00006473979,0.0010804639],"genre_scores_gemma":[0.9976665,0.000087058674,0.0019843217,0.000012415843,0.0000036067509,0.000002977612,0.000058990157,0.000014773624,0.00016940813],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999629,0.000009533974,0.0000013040118,0.000006896256,0.000008090345,0.000011181757],"domain_scores_gemma":[0.9997367,0.00009586611,0.00006745024,0.000031564367,0.000020444211,0.000047918318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021965096,0.00028401546,0.00017525292,0.0002235523,0.0002891967,0.00046766046,0.0004460589,0.0003455611,0.0007361738],"category_scores_gemma":[0.0009814024,0.00016680062,0.00027117739,0.00026931887,0.00032532105,0.0006806977,0.000374216,0.000548033,0.00007060176],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032627245,0.00017438759,0.1472426,0.00014583001,0.00018188638,0.00075622747,0.0007212561,0.6922683,0.1300322,0.009848184,0.0006885451,0.017614286],"study_design_scores_gemma":[0.000043129316,0.00007027235,0.063729696,0.000012866393,0.000029710523,0.00010891502,0.00012755649,0.91717756,0.014345687,0.0035193288,0.00079803175,0.000037185328],"about_ca_topic_score_codex":0.008911872,"about_ca_topic_score_gemma":0.0060785706,"teacher_disagreement_score":0.008911872,"about_ca_system_score_codex":0.0005316746,"about_ca_system_score_gemma":0.00032836286,"threshold_uncertainty_score":0.017719984},"labels":[],"label_agreement":null},{"id":"W1995303605","doi":"10.1086/338279","title":"Spectroscopic Analysis of the DAB White Dwarf PG 1115+166: An Unresolved DA + DB Degenerate Binary","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Degenerate energy levels; Spectral line; Binary number; Helium; Line (geometry); Homogeneous; Radial velocity; Effective temperature; Binary system","score_opus":0.018712768428189572,"score_gpt":0.23463168859043707,"score_spread":0.2159189201622475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995303605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987078,0.00008717997,0.00017180583,0.000014536286,0.0000028960167,0.000003948703,0.00007687173,0.0000063678262,0.00092860044],"genre_scores_gemma":[0.9990409,0.000039962368,0.00029455125,0.000013480799,0.0000038376,0.0000020010818,0.0002699587,0.0000021204075,0.000333255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999312,0.000004630284,0.0000046895307,0.000022078202,0.000023121454,0.000014298054],"domain_scores_gemma":[0.9998845,0.000009147404,0.000028906616,0.0000109421735,0.000010900542,0.00005562642],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006702587,0.00024316167,0.00029874837,0.0007805984,0.00061620085,0.0003104154,0.0001552193,0.00023849714,0.0007594375],"category_scores_gemma":[0.00019764053,0.00012628405,0.00008329095,0.0005787384,0.00024350877,0.00010773485,0.0003895004,0.0001895572,0.00038425287],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006212195,0.00018661813,0.5818308,0.00014523389,0.0000486972,0.0057291323,0.0007003405,0.0005545065,0.38108552,0.00086571526,0.00043607474,0.027796214],"study_design_scores_gemma":[0.000015054575,0.0003188055,0.97429216,0.000007666199,0.000029883939,0.006450935,0.00034320288,0.00078465237,0.014410841,0.00021790527,0.0031199963,0.000008853495],"about_ca_topic_score_codex":0.0010467207,"about_ca_topic_score_gemma":0.0015054861,"teacher_disagreement_score":0.0010467207,"about_ca_system_score_codex":0.00026511023,"about_ca_system_score_gemma":0.000105691484,"threshold_uncertainty_score":0.0025405288},"labels":[],"label_agreement":null},{"id":"W1995361242","doi":"10.1086/318415","title":"High‐Energy Gamma‐Ray Observations of the Crab Nebula and Pulsar with the Solar Tower Atmospheric Cerenkov Effect Experiment","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Heliostat; Cherenkov radiation; Crab Pulsar; Pulsar; Crab Nebula; Flux (metallurgy); Telescope; Gamma ray; Tower","score_opus":0.005765714790718203,"score_gpt":0.193874330009653,"score_spread":0.18810861521893482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995361242","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98807585,0.0003025138,0.0038020834,0.00007644823,0.000016662842,0.000060592898,0.001827162,0.00019064774,0.0056482027],"genre_scores_gemma":[0.98138535,0.00021123816,0.012927948,0.000095254916,0.00002518243,0.000051006515,0.0034989163,0.000054497115,0.0017506139],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9996867,0.000038981645,0.000012007998,0.00006465964,0.00015154142,0.00004601056],"domain_scores_gemma":[0.99948126,0.00007826514,0.000109720444,0.00012020545,0.00009661432,0.00011391921],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056496245,0.00021119474,0.00024531942,0.0007448512,0.00047037198,0.00040186394,0.00036815752,0.0003252922,0.0010196257],"category_scores_gemma":[0.0005047707,0.00025198676,0.0002882113,0.0008373871,0.00024475428,0.00029437782,0.00071710144,0.00043752205,0.0001853975],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016615834,0.00040340872,0.36708534,0.00013708467,0.0003041487,0.0006066437,0.00032331288,0.0025828192,0.5940664,0.0013261897,0.0041612023,0.027341822],"study_design_scores_gemma":[0.00017888246,0.0006422292,0.94692343,0.000012788414,0.000055576143,0.00091707945,0.000053369433,0.0038389326,0.03961142,0.00023839634,0.0074928375,0.000034933833],"about_ca_topic_score_codex":0.0021365292,"about_ca_topic_score_gemma":0.008377121,"teacher_disagreement_score":0.0021365292,"about_ca_system_score_codex":0.00030513853,"about_ca_system_score_gemma":0.00035799798,"threshold_uncertainty_score":0.004248202},"labels":[],"label_agreement":null},{"id":"W1995374968","doi":"10.1086/374734","title":"Substructure in the Andromeda Galaxy Globular Cluster System","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Globular cluster; Substructure; Andromeda Galaxy; Galaxy; Interacting galaxy; Cluster (spacecraft); Galaxy merger; Galaxy cluster; Andromeda","score_opus":0.005151321727239435,"score_gpt":0.19504448230056134,"score_spread":0.18989316057332192,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995374968","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965843,0.00030175594,0.0002762864,0.000042841213,0.000002405466,0.000005965447,0.00031130147,0.00003471737,0.002440394],"genre_scores_gemma":[0.9984126,0.000081059574,0.0005207454,0.000010162355,0.0000021063145,0.0000022473237,0.00042731388,0.000006700476,0.00053687004],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988854,0.00002073996,0.000006516852,0.000040396633,0.000025339792,0.00001832543],"domain_scores_gemma":[0.9997198,0.00005420101,0.00009756675,0.000033162567,0.000029928415,0.00006534786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001658739,0.0002064022,0.0002065532,0.0010760337,0.00059843314,0.0008583586,0.00032108187,0.00025694811,0.0026469324],"category_scores_gemma":[0.0008785408,0.00011197433,0.00014125758,0.00095835474,0.00041086992,0.00033534758,0.0005817131,0.00016193537,0.00044987048],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044820842,0.00007072943,0.91711754,0.00010522426,0.00014175577,0.0007948105,0.0011999821,0.018964127,0.022037497,0.009237076,0.0013640211,0.028519098],"study_design_scores_gemma":[0.000028108629,0.00009285243,0.9565329,0.000025945212,0.000073394614,0.00068666064,0.00078731735,0.033335764,0.0015560492,0.0038536508,0.0029860935,0.000041330368],"about_ca_topic_score_codex":0.021935795,"about_ca_topic_score_gemma":0.019296419,"teacher_disagreement_score":0.021935795,"about_ca_system_score_codex":0.00048795526,"about_ca_system_score_gemma":0.00023053946,"threshold_uncertainty_score":0.043616235},"labels":[],"label_agreement":null},{"id":"W1995478073","doi":"10.1086/503193","title":"The Large‐ and Small‐Scale Structures of Dust in the Star‐forming Perseus Molecular Cloud","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":219,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Molecular cloud; Cosmic dust; Cloud computing; Interstellar cloud; Dark nebula; Interstellar medium; Emission spectrum","score_opus":0.005314308985852046,"score_gpt":0.21378655090642082,"score_spread":0.20847224192056876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995478073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97404116,0.0011340089,0.00015151614,0.0029335795,0.00083327375,0.000029628029,0.0007107168,0.0000714074,0.02009468],"genre_scores_gemma":[0.9826124,0.00055378757,0.00011308049,0.0002155019,0.0006920776,0.0000057035836,0.0005969779,0.000026230131,0.015184347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986243,0.000016003944,0.000007595862,0.000033139982,0.00005839363,0.000022353068],"domain_scores_gemma":[0.9971482,0.0005654944,0.0002811141,0.00010365634,0.0014875085,0.00041397815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003180241,0.00012936497,0.00023259477,0.00078093325,0.00074335496,0.0009485323,0.00028696048,0.0005743508,0.01475998],"category_scores_gemma":[0.00284356,0.00011777254,0.000081096296,0.00041362018,0.00036474565,0.0005373133,0.00030621214,0.00022169587,0.002235346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020764999,0.00021457745,0.59855354,0.0011726256,0.000089498935,0.00433385,0.0017247258,0.0034055049,0.1025845,0.0057522813,0.102135345,0.1779571],"study_design_scores_gemma":[0.00010714471,0.0001754145,0.94836843,0.00006466095,0.000037354814,0.0007324869,0.0010155981,0.0024529693,0.009684179,0.001539311,0.03579819,0.000024201787],"about_ca_topic_score_codex":0.0038757077,"about_ca_topic_score_gemma":0.00552613,"teacher_disagreement_score":0.01475998,"about_ca_system_score_codex":0.00042255904,"about_ca_system_score_gemma":0.00037558877,"threshold_uncertainty_score":0.049377084},"labels":[],"label_agreement":null},{"id":"W1995573488","doi":"10.1086/312758","title":"A Glitch in an Anomalous X-Ray Pulsar","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Glitch; Magnetar; Neutron star; Vela; Radio telescope; Moment of inertia; Binary pulsar","score_opus":0.010680891977692354,"score_gpt":0.30959616045375843,"score_spread":0.2989152684760661,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995573488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99908197,0.00009792496,0.0002056811,0.000036481466,0.000019877176,0.0000045919815,0.00010321259,0.000027351953,0.00042285252],"genre_scores_gemma":[0.9986665,0.00010229185,0.0006023381,0.000055702378,0.000048566828,0.0000057707134,0.00032435975,0.000007663377,0.0001868482],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999918,0.0000077237555,0.000007675483,0.000028068656,0.000020901549,0.00001769515],"domain_scores_gemma":[0.99961746,0.000043972777,0.00018897484,0.00004597842,0.00003474561,0.00006882158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014979097,0.00021211621,0.00019121294,0.00054549833,0.0003638888,0.00035464202,0.00016336358,0.000392224,0.0004433896],"category_scores_gemma":[0.0005488372,0.00012965765,0.00017618215,0.000325109,0.00041595884,0.00018968286,0.0006621204,0.000382637,0.00017209239],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006213586,0.000075450196,0.8143437,0.00011005192,0.00012735165,0.0133106345,0.0007334553,0.0006083211,0.14560494,0.000476726,0.0011372475,0.022850834],"study_design_scores_gemma":[0.00001824822,0.00048293202,0.97319454,0.0000134726,0.000044209974,0.013667757,0.0001796924,0.0010541041,0.0077569582,0.00021091179,0.0033566866,0.000020437954],"about_ca_topic_score_codex":0.0006238195,"about_ca_topic_score_gemma":0.0011431817,"teacher_disagreement_score":0.0006238195,"about_ca_system_score_codex":0.00012821353,"about_ca_system_score_gemma":0.000071091024,"threshold_uncertainty_score":0.0014833212},"labels":[],"label_agreement":null},{"id":"W1995609620","doi":"10.1086/505903","title":"The<i>Spitzer</i>c2d Survey of Nearby Dense Cores. III. Low‐Mass Star Formation in a Small Group, L1251B","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Protostar; Star formation; Nebula; Emission nebula; Interferometry; Bipolar outflow; H II region","score_opus":0.01205152051478521,"score_gpt":0.21971940568074144,"score_spread":0.20766788516595625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995609620","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961921,0.00029670144,0.00008538769,0.000037316244,0.0000022110862,0.000014841849,0.0018532367,0.000015134824,0.0015029624],"genre_scores_gemma":[0.98924166,0.0003040924,0.00050381134,0.000050465027,0.000013918108,0.000020068012,0.008555336,0.0000067421265,0.0013039638],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999068,0.0000059506337,0.0000060311568,0.000019906985,0.000029697836,0.000031569794],"domain_scores_gemma":[0.9996698,0.000011686179,0.00010489094,0.00001821037,0.000037326437,0.000158113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013286127,0.00018401814,0.00018857059,0.002430183,0.00040240062,0.00036720058,0.00025357306,0.00014796638,0.0012788257],"category_scores_gemma":[0.00023487523,0.00011414198,0.00017025687,0.0009365545,0.00015793259,0.00018671756,0.0004864181,0.00015350852,0.0005148609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010384322,0.000063369334,0.9711505,0.000052170803,0.000045499535,0.00015373678,0.00042923065,0.0001036066,0.013215525,0.0001309182,0.0015751658,0.012976393],"study_design_scores_gemma":[0.000003311504,0.000015081518,0.9983504,0.0000039025117,0.0000055631585,0.00006311179,0.000053594107,0.000048691632,0.00020724289,0.000009845585,0.0012380268,0.0000013619137],"about_ca_topic_score_codex":0.02473262,"about_ca_topic_score_gemma":0.05196002,"teacher_disagreement_score":0.02473262,"about_ca_system_score_codex":0.00041857,"about_ca_system_score_gemma":0.00022281581,"threshold_uncertainty_score":0.04917735},"labels":[],"label_agreement":null},{"id":"W1995654386","doi":"10.1088/0004-637x/730/2/97","title":"COMPOSITIONALLY DRIVEN CONVECTION IN THE OCEANS OF ACCRETING NEUTRON STARS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Convection; Buoyancy; Physics; Diffusion; Convective mixing; Flux (metallurgy); Accretion (finance); Neutron star; Water mass; Astrophysics; Atmospheric sciences; Geology; Thermodynamics; Chemistry; Oceanography","score_opus":0.016452289500014997,"score_gpt":0.22563360214084535,"score_spread":0.20918131264083034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995654386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993725,0.00012855856,0.0038230864,0.00012477754,0.000013829639,0.000008044969,0.000052784282,0.000032364507,0.0020915305],"genre_scores_gemma":[0.9984848,0.000081858,0.0008474299,0.00002018625,0.000006466845,0.000006013867,0.00004758298,0.0000147047995,0.00049111666],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995184,0.0000103408065,0.0000040494488,0.000009019755,0.000008735771,0.000016022113],"domain_scores_gemma":[0.99987245,0.000031144144,0.000033928638,0.000010033851,0.000017604516,0.00003480781],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014659013,0.00035812875,0.00028951315,0.00035981534,0.0005497505,0.0007222046,0.00038381832,0.00053567206,0.0007531515],"category_scores_gemma":[0.0008265278,0.00032189378,0.0005465236,0.00022326154,0.00090131315,0.00073382637,0.0008685241,0.00034890499,0.00008663057],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035813497,0.00010789876,0.056795385,0.00009125055,0.00008915033,0.0007735302,0.00042803687,0.8482693,0.06760927,0.020131083,0.00021846445,0.005128411],"study_design_scores_gemma":[0.00014930376,0.00011129713,0.02284116,0.000016533031,0.000030691976,0.00012340376,0.00019795292,0.96064633,0.0059551448,0.009378484,0.00050644536,0.00004322314],"about_ca_topic_score_codex":0.010138688,"about_ca_topic_score_gemma":0.0048499852,"teacher_disagreement_score":0.010138688,"about_ca_system_score_codex":0.00088346587,"about_ca_system_score_gemma":0.00073905475,"threshold_uncertainty_score":0.020159364},"labels":[],"label_agreement":null},{"id":"W1995670451","doi":"10.1086/502960","title":"First Detection of Na<scp>i</scp>D Lines in High‐Redshift Damped Lyα Systems","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Redshift; Astrophysics; Absorption (acoustics); Absorption spectroscopy; Spectral line; Quasar; Rest frame; Galaxy; Optics; Astronomy","score_opus":0.006780725740835955,"score_gpt":0.20871906001286766,"score_spread":0.2019383342720317,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995670451","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99777156,0.00017941378,0.0005719537,0.000059342445,0.000007106117,0.0000098479695,0.00009490794,0.00006468352,0.0012410919],"genre_scores_gemma":[0.9989712,0.000043797707,0.00064864795,0.00004353423,0.000010966441,0.000004602551,0.00011041984,0.000006814687,0.00016002762],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984527,0.000008524292,0.000008759642,0.000048990983,0.0000458625,0.000042594726],"domain_scores_gemma":[0.9995171,0.000046460136,0.0001532615,0.000054361655,0.00008148286,0.00014735559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019026396,0.00030716826,0.00025340656,0.0007797575,0.0005605822,0.0005972329,0.0005166299,0.000520925,0.0007926267],"category_scores_gemma":[0.0005161884,0.00039369435,0.00016647918,0.00045425634,0.00055145455,0.00035447354,0.0007175277,0.0006182584,0.00022815878],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029597722,0.000101260695,0.6044184,0.00010215899,0.00010219466,0.0011053813,0.000654056,0.00023311815,0.37548262,0.00069069973,0.00065936125,0.016154787],"study_design_scores_gemma":[0.00002912079,0.00014214819,0.97811526,0.00000856121,0.000037284444,0.0007700231,0.00009368178,0.00070611347,0.01739942,0.0001453258,0.0025406342,0.000012518713],"about_ca_topic_score_codex":0.0017215909,"about_ca_topic_score_gemma":0.0028895936,"teacher_disagreement_score":0.0017215909,"about_ca_system_score_codex":0.0005214921,"about_ca_system_score_gemma":0.00012417953,"threshold_uncertainty_score":0.0037837625},"labels":[],"label_agreement":null},{"id":"W1995674593","doi":"10.1088/0004-637x/710/1/797","title":"EXTINCTION AND DISTANCE TO ANOMALOUS X-RAY PULSARS FROM X-RAY SCATTERING HALOS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Extinction (optical mineralogy); Line-of-sight; Pulsar; Halo; Scattering; Brightness; Spectral line; Line (geometry); Surface brightness; Astronomy; Optics; Geometry; Galaxy","score_opus":0.007911294446982227,"score_gpt":0.22081593188120427,"score_spread":0.21290463743422205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995674593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937063,0.00005725333,0.00023660861,0.000007987392,4.372672e-7,8.2063167e-7,0.000029692612,0.000007973768,0.00028862775],"genre_scores_gemma":[0.99967396,0.000042183892,0.00010129316,0.0000025265288,0.0000026513726,6.3707137e-7,0.0001365053,0.0000034768905,0.000036832836],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999026,0.00001363907,0.000007380081,0.000020053201,0.000029087996,0.0000271766],"domain_scores_gemma":[0.99858296,0.00037926534,0.0005039979,0.00014832059,0.00014154252,0.0002439158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035643912,0.00029134116,0.00018199922,0.0013063612,0.00022621815,0.00067291054,0.00022366169,0.00015166092,0.00071736495],"category_scores_gemma":[0.0017845544,0.00015442962,0.0002466772,0.0006510795,0.00048290726,0.0003593524,0.0010364046,0.00020329184,0.00013499329],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001316029,0.000015464335,0.9770156,0.000016416532,0.00010332889,0.00017282959,0.00029176802,0.00593604,0.010870583,0.00079160824,0.00007521023,0.0045795944],"study_design_scores_gemma":[0.000010289702,0.000036901554,0.98876023,0.0000062240856,0.000026414085,0.00030231048,0.00014490249,0.008125543,0.0012383463,0.0011155873,0.00022483683,0.000008475767],"about_ca_topic_score_codex":0.0013716461,"about_ca_topic_score_gemma":0.001384595,"teacher_disagreement_score":0.0013716461,"about_ca_system_score_codex":0.00022896184,"about_ca_system_score_gemma":0.0001084508,"threshold_uncertainty_score":0.0027272701},"labels":[],"label_agreement":null},{"id":"W1995709019","doi":"10.1088/0004-637x/783/1/4","title":"INFLUENCE OF STELLAR MULTIPLICITY ON PLANET FORMATION. I. EVIDENCE OF SUPPRESSED PLANET FORMATION DUE TO STELLAR COMPANIONS WITHIN 20 AU AND VALIDATION OF FOUR PLANETS FROM THE<i>KEPLER</i>MULTIPLE PLANET CANDIDATES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planet; Physics; Stars; Astrophysics; Astronomy; Planetary system; Terrestrial planet; Kepler","score_opus":0.017428339601099477,"score_gpt":0.2260701506270898,"score_spread":0.20864181102599033,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995709019","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992112,0.00008772201,0.0002626805,0.00000643035,0.0000013179424,0.0000017115453,0.000075841155,0.000009288775,0.0003437288],"genre_scores_gemma":[0.99956506,0.000016748956,0.00020904306,0.000002252898,0.0000014845201,0.0000019036818,0.00014637115,0.0000031048328,0.000054005955],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999134,0.00015831608,0.00011939036,0.00026317744,0.00022137177,0.000103791775],"domain_scores_gemma":[0.99102134,0.004245287,0.002932178,0.0007237988,0.0005411764,0.00053624593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012101468,0.0002234956,0.00038332777,0.0019290679,0.00045182757,0.00070748554,0.0003512611,0.00025239144,0.00082465145],"category_scores_gemma":[0.008434254,0.00017739736,0.00025087135,0.00067766296,0.00044957633,0.00051916233,0.00094609,0.00023255375,0.00019979732],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001904418,0.000012612397,0.98443836,0.000019511934,0.00004237999,0.000094707975,0.00009781382,0.00048289672,0.010526472,0.0000837556,0.0000350328,0.003976013],"study_design_scores_gemma":[0.0000049306964,0.00010237908,0.9870767,0.0000043232344,0.0000307345,0.000541954,0.000086092696,0.0035660362,0.008260723,0.00009500755,0.00022488725,0.000006221339],"about_ca_topic_score_codex":0.0010066825,"about_ca_topic_score_gemma":0.0013718152,"teacher_disagreement_score":0.0019290679,"about_ca_system_score_codex":0.00027439528,"about_ca_system_score_gemma":0.000120655845,"threshold_uncertainty_score":0.006399989},"labels":[],"label_agreement":null},{"id":"W1995711731","doi":"10.1086/317828","title":"Implementing Feedback in Simulations of Galaxy Formation: A Survey of Methods","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":215,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Alberta; Western University","funders":"","keywords":"Physics; Star formation; Smoothed-particle hydrodynamics; Astrophysics; Galaxy; Radiative cooling; Galaxy formation and evolution; Supernova; Redshift; Gravitation; Astronomy","score_opus":0.02456323424316442,"score_gpt":0.3064932384948247,"score_spread":0.28193000425166026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995711731","genre_codex":"methods","genre_gemma":"review","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"review","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.026768766,0.005909564,0.9555603,0.0006044762,0.00018013554,0.0002714148,0.00039342817,0.00509642,0.0052154106],"genre_scores_gemma":[0.36133063,0.013274312,0.6170451,0.00034103822,0.0002981862,0.001108231,0.00051691604,0.00269995,0.0033856288],"study_design_codex":"simulation_or_modeling","study_design_gemma":"not_applicable","domain_scores_codex":[0.9982132,0.0008712652,0.00014925934,0.00019621864,0.00046564365,0.00010445361],"domain_scores_gemma":[0.99386334,0.0037242477,0.00042748929,0.0011276234,0.00058333867,0.00027399862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028881347,0.0017516245,0.0018938711,0.0013072061,0.000962489,0.0019808344,0.004545302,0.0021981061,0.0032755611],"category_scores_gemma":[0.009702161,0.0014919718,0.0015328462,0.0016823659,0.0013488812,0.002484508,0.00209613,0.0022876358,0.0010658219],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001831394,0.00021003805,0.0049109934,0.00086822885,0.00032632565,0.000119551056,0.00029766405,0.8594394,0.002802228,0.03481489,0.0012527667,0.09477477],"study_design_scores_gemma":[0.000081049315,0.00005577252,0.00034107227,0.00011351853,0.000036316556,0.00004094161,0.000035722845,0.97697234,0.0014061142,0.015695086,0.005169077,0.00005286165],"about_ca_topic_score_codex":0.014742522,"about_ca_topic_score_gemma":0.0091021685,"teacher_disagreement_score":0.014742522,"about_ca_system_score_codex":0.0018978801,"about_ca_system_score_gemma":0.0013642892,"threshold_uncertainty_score":0.029313445},"labels":[],"label_agreement":null},{"id":"W1995743228","doi":"10.1086/529419","title":"Globular Clusters and X‐Ray Point Sources in Centaurus A (NGC 5128)","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Centaurus A; Galaxy; Astronomy; Luminosity; Population; Elliptical galaxy; RADIUS; Point source; Star cluster; Radio galaxy; Medicine","score_opus":0.006486235721614133,"score_gpt":0.19343984132553177,"score_spread":0.18695360560391763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995743228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997396,0.00002155393,0.000022656133,0.000003621892,7.137357e-7,0.0000011998164,0.000061526756,0.0000043604564,0.00014474275],"genre_scores_gemma":[0.9995252,0.000024443216,0.0001159529,0.000003270101,0.000003769179,0.0000025681518,0.0002160838,9.90241e-7,0.000107740685],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999806,0.000018276465,0.000020245352,0.00006605603,0.000041451767,0.00004792913],"domain_scores_gemma":[0.9991155,0.00010579373,0.00040811725,0.00013263382,0.00004313244,0.00019473612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018761952,0.00027528123,0.00020829818,0.0016909835,0.0004731094,0.0005593158,0.00029189693,0.00030431114,0.0012532598],"category_scores_gemma":[0.0008545944,0.00022755135,0.00015231874,0.0009796722,0.000402571,0.0003304695,0.0009856565,0.00016327061,0.00035713523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017710678,0.00003276727,0.98078364,0.00001618806,0.000031227235,0.00038483526,0.00042954675,0.00022370573,0.012506134,0.00010333207,0.00011702806,0.0051945853],"study_design_scores_gemma":[0.000006393913,0.00003798997,0.9987086,0.0000041278972,0.000009969997,0.00034706108,0.000111286645,0.00017349944,0.0003787273,0.000049505325,0.00016842206,0.0000042787856],"about_ca_topic_score_codex":0.0063311746,"about_ca_topic_score_gemma":0.010276335,"teacher_disagreement_score":0.0063311746,"about_ca_system_score_codex":0.0002733409,"about_ca_system_score_gemma":0.00012522929,"threshold_uncertainty_score":0.01258862},"labels":[],"label_agreement":null},{"id":"W1995889176","doi":"10.1088/0004-637x/730/2/128","title":"AN IMPROVED SPECTROSCOPIC ANALYSIS OF DA WHITE DWARFS FROM THE SLOAN DIGITAL SKY SURVEY DATA RELEASE 4","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":442,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"White dwarf; Sky; Stars; Brown dwarf; Effective temperature; Sampling (signal processing); Spectroscopy","score_opus":0.03484882335798826,"score_gpt":0.25352254382532646,"score_spread":0.2186737204673382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995889176","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8871071,0.000616644,0.051749192,0.00036986044,0.00007312294,0.000170335,0.04489656,0.0033489699,0.011668176],"genre_scores_gemma":[0.8110073,0.00033791288,0.0745022,0.00017541544,0.00013035818,0.00014088213,0.10720838,0.00066494563,0.005832626],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99939406,0.000088931425,0.00006262373,0.0001292302,0.00024383959,0.00008124643],"domain_scores_gemma":[0.9987326,0.00009774519,0.00026374042,0.0003163485,0.00047447343,0.00011512235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011194902,0.00053859566,0.00032117893,0.0040011047,0.00043556327,0.0005667201,0.00036502862,0.00014366464,0.0025746075],"category_scores_gemma":[0.0014587548,0.00019230395,0.0005113871,0.0017253426,0.00009934135,0.00030942765,0.0008272585,0.0002704209,0.0016820586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027149418,0.00013137663,0.78627145,0.00022766272,0.00026208416,0.00026023018,0.00038630457,0.009553543,0.06937406,0.0018782606,0.023112869,0.1082707],"study_design_scores_gemma":[0.000031960528,0.00005097069,0.94305074,0.000015167132,0.00006172526,0.00017534257,0.00008110213,0.012729666,0.007336344,0.00049694633,0.03594121,0.000028854334],"about_ca_topic_score_codex":0.023273887,"about_ca_topic_score_gemma":0.032511503,"teacher_disagreement_score":0.023273887,"about_ca_system_score_codex":0.0004554001,"about_ca_system_score_gemma":0.0006058343,"threshold_uncertainty_score":0.046276808},"labels":[],"label_agreement":null},{"id":"W1995898085","doi":"10.1088/0004-637x/756/1/72","title":"A FULLY IDENTIFIED SAMPLE OF AEGIS20 MICROJANSKY RADIO SOURCES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Redshift; Astrophysics; Physics; Galaxy; Active galactic nucleus; Astronomy; Sample (material); Radio galaxy","score_opus":0.009260675265663688,"score_gpt":0.2140502154126649,"score_spread":0.2047895401470012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995898085","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9876274,0.00019607849,0.00096690183,0.00003287405,0.000005039274,0.00005715315,0.0046017645,0.00007370157,0.0064390395],"genre_scores_gemma":[0.9690766,0.00030340804,0.0028304793,0.00008555022,0.000026530342,0.00007061694,0.024699302,0.000028318967,0.0028791563],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997836,0.000018238306,0.00002358421,0.000060490907,0.000047446996,0.000066716646],"domain_scores_gemma":[0.999589,0.00003847442,0.000106647465,0.000095047086,0.00006580932,0.000105032304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003061981,0.00032686116,0.0002727612,0.0014252892,0.00026917155,0.00037828647,0.0002619537,0.000154197,0.0033028023],"category_scores_gemma":[0.0005809717,0.00022483229,0.00023894985,0.00074072793,0.00012724963,0.00040430686,0.0010113053,0.00013131423,0.0013795629],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005674706,0.00022540595,0.7850343,0.00011911557,0.00012881847,0.0008233441,0.0007557383,0.0006259856,0.11667018,0.0011882257,0.004174551,0.08968677],"study_design_scores_gemma":[0.000011973622,0.00004667988,0.99209994,0.000007672756,0.000017129436,0.0003350349,0.000081904414,0.00019807804,0.0021686982,0.000078215926,0.0049502887,0.000004284418],"about_ca_topic_score_codex":0.0031365273,"about_ca_topic_score_gemma":0.008353629,"teacher_disagreement_score":0.0033028023,"about_ca_system_score_codex":0.000210449,"about_ca_system_score_gemma":0.00021953581,"threshold_uncertainty_score":0.011049032},"labels":[],"label_agreement":null},{"id":"W1995947764","doi":"10.1086/506380","title":"Distances to Anomalous X‐Ray Pulsars Using Red Clump Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Pulsar; Red clump; Stars; Extinction (optical mineralogy); Spiral galaxy; Giant star; Spectroscopy; Measure (data warehouse); Magnetic field","score_opus":0.012820190033807048,"score_gpt":0.23976704579308714,"score_spread":0.2269468557592801,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995947764","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99805474,0.000120194825,0.0006491171,0.00001862103,0.0000042215634,0.0000015451715,0.00017334831,0.000017220029,0.0009610832],"genre_scores_gemma":[0.99877673,0.00004979176,0.0007373336,0.000005888773,0.000009318658,0.0000019307467,0.0002900075,0.0000048396278,0.00012405722],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997898,0.000031337302,0.000020351317,0.00007641952,0.000050628227,0.000031502586],"domain_scores_gemma":[0.9970391,0.0005365447,0.001638849,0.00020647663,0.00027254524,0.00030660682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004713561,0.00023500403,0.00013586496,0.0017172546,0.00024682257,0.00076996104,0.00025922127,0.00026317133,0.0006490459],"category_scores_gemma":[0.0028250727,0.00014947822,0.000118414646,0.0008566191,0.00025711794,0.00055137684,0.00069466984,0.00031913238,0.00028185907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000961486,0.0000104694645,0.9834071,0.000021744207,0.000042822296,0.000063879066,0.00021412986,0.0014239951,0.004601408,0.00076832774,0.00016521443,0.009184762],"study_design_scores_gemma":[0.000008797897,0.00006348347,0.9919105,0.000010670877,0.00002249771,0.00033869394,0.00013542842,0.0036156168,0.0020320269,0.000914649,0.0009373448,0.00001031361],"about_ca_topic_score_codex":0.0010937132,"about_ca_topic_score_gemma":0.0017320588,"teacher_disagreement_score":0.0017172546,"about_ca_system_score_codex":0.00020686106,"about_ca_system_score_gemma":0.00008271978,"threshold_uncertainty_score":0.0024927855},"labels":[],"label_agreement":null},{"id":"W1995949099","doi":"10.1088/0004-637x/717/2/1084","title":"NEAR-INFRARED THERMAL EMISSION FROM THE HOT JUPITER TrES-2b: GROUND-BASED DETECTION OF THE SECONDARY ECLIPSE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Eclipse; Physics; Infrared; Black-body radiation; Astrophysics; Brightness temperature; Hot Jupiter; Planet; Astronomy; Circular orbit; Atmosphere (unit); Radiance; Brightness; Exoplanet; Optics; Meteorology; Radiation","score_opus":0.007173794186601434,"score_gpt":0.20472046875660319,"score_spread":0.19754667457000175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995949099","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954999,0.00015214515,0.00027377327,0.000025327265,0.000005800364,0.000009921497,0.00040411417,0.00006710478,0.0035618222],"genre_scores_gemma":[0.99778783,0.00005526168,0.00059424405,0.000029025783,0.000011787353,0.000007703113,0.0010914129,0.000019314424,0.00040333607],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999037,0.0000038014882,0.0000025475856,0.00002818967,0.000032488904,0.00002928331],"domain_scores_gemma":[0.99971706,0.000020488369,0.000069574846,0.00002502178,0.000049741488,0.00011815254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010849755,0.0002765953,0.00027636232,0.0006578508,0.0003714389,0.00035729,0.00034034954,0.0003670912,0.0011426606],"category_scores_gemma":[0.00022458783,0.00018030165,0.00023841369,0.00040599486,0.00022327242,0.00015801046,0.0003857836,0.00040169753,0.00041562982],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076651725,0.00016351143,0.34455416,0.00015750765,0.00009526192,0.0013095717,0.00061579293,0.00063010777,0.6375598,0.00014613062,0.0016221073,0.012379639],"study_design_scores_gemma":[0.0000162847,0.00012382469,0.9877215,0.000011111154,0.000019771162,0.0006518171,0.00008483209,0.00091957074,0.009058526,0.000028307839,0.001357316,0.0000071761583],"about_ca_topic_score_codex":0.0030877022,"about_ca_topic_score_gemma":0.009006884,"teacher_disagreement_score":0.0030877022,"about_ca_system_score_codex":0.00025908017,"about_ca_system_score_gemma":0.00009978833,"threshold_uncertainty_score":0.006139457},"labels":[],"label_agreement":null},{"id":"W1995965054","doi":"10.1088/0004-637x/795/1/82","title":"THE Hα PROFILES OF Be SHELL STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Deutsche Forschungsgemeinschaft; University of Cambridge","keywords":"Physics; Astrophysics; Stars; Degeneracy (biology); Inclination angle; Observable; Spectral line; Line (geometry); Shell (structure); Star (game theory); Range (aeronautics); Series (stratigraphy); Function (biology); Work (physics); Geometry; Astronomy","score_opus":0.009283112756360703,"score_gpt":0.23067061564396213,"score_spread":0.22138750288760142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1995965054","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9865008,0.00005132517,0.009567257,0.000022005295,0.000007498987,0.000018329076,0.00058567716,0.00023064113,0.0030164497],"genre_scores_gemma":[0.99274546,0.000047409372,0.0048370594,0.000008513573,0.0000032696905,0.000012629672,0.0015728386,0.00005374415,0.0007190144],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998592,0.00002048718,0.0000068239847,0.00004541969,0.000041673207,0.000026402622],"domain_scores_gemma":[0.999658,0.000047248872,0.000048625156,0.00006322929,0.00012325539,0.000059656897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035680275,0.00032431772,0.00038315824,0.0006543962,0.00038004154,0.0005595392,0.00040995557,0.0003983505,0.0009453866],"category_scores_gemma":[0.00074296194,0.00025430936,0.0004948883,0.00044137618,0.0002757012,0.00046424707,0.00025881676,0.00040731777,0.000527448],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067248737,0.0001992465,0.29550308,0.000112634414,0.00023398195,0.0004926284,0.00067226595,0.6073113,0.06184295,0.0055155847,0.0013921193,0.026051769],"study_design_scores_gemma":[0.000061345185,0.00024507556,0.24160144,0.000015401652,0.000048248894,0.00051034015,0.0002753823,0.73599917,0.015796151,0.0016415538,0.003754284,0.00005149919],"about_ca_topic_score_codex":0.003657404,"about_ca_topic_score_gemma":0.0026461945,"teacher_disagreement_score":0.003657404,"about_ca_system_score_codex":0.00082197465,"about_ca_system_score_gemma":0.00020051777,"threshold_uncertainty_score":0.0072722435},"labels":[],"label_agreement":null},{"id":"W1996041070","doi":"10.1086/510550","title":"[Fe<scp>ii</scp>] and H<sub>2</sub>Filaments in the Supernova Remnant G11.2−0.3: Supernova Ejecta and Presupernova Circumstellar Wind","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Supernova remnant; Cassiopeia A; Ejecta; Supernova; Line (geometry); Near-Earth supernova; Supergiant; Proper motion","score_opus":0.010631864074039215,"score_gpt":0.2239013380442156,"score_spread":0.2132694739701764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996041070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99966323,0.00006890196,0.000028830107,0.0000074698883,6.432771e-7,0.0000012898176,0.00004522132,0.0000039623123,0.00018056351],"genre_scores_gemma":[0.99956137,0.000037976275,0.00006905716,0.000010594965,0.0000044242183,0.0000018933401,0.0001927357,0.0000023205696,0.000119639444],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999522,0.0000045016013,0.0000030478711,0.000014558813,0.000009357658,0.000016233631],"domain_scores_gemma":[0.9998022,0.000025043415,0.00009288301,0.0000075746143,0.00001540222,0.00005701227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011451865,0.00021388022,0.00015118804,0.0005801227,0.00021000681,0.00035128885,0.00018726279,0.00028172688,0.00069077185],"category_scores_gemma":[0.00021918486,0.00020160743,0.00014539751,0.00025495805,0.0002513394,0.00013483324,0.00025541423,0.00018806245,0.00014301842],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086390914,0.00009034602,0.9273,0.00003234346,0.00009888891,0.0032379464,0.0002289973,0.00049116457,0.06242889,0.00008096141,0.00027271602,0.004873793],"study_design_scores_gemma":[0.000003998448,0.000030020894,0.9983375,0.0000017840601,0.000011361713,0.0006217037,0.000033023647,0.00019919132,0.00066816853,0.0000116343435,0.00007964412,0.0000020654998],"about_ca_topic_score_codex":0.006668764,"about_ca_topic_score_gemma":0.008949353,"teacher_disagreement_score":0.006668764,"about_ca_system_score_codex":0.00028954734,"about_ca_system_score_gemma":0.00007262238,"threshold_uncertainty_score":0.013259947},"labels":[],"label_agreement":null},{"id":"W1996151155","doi":"10.1088/0004-637x/745/2/178","title":"DIRECT EVIDENCE FOR TERMINATION OF OBSCURED STAR FORMATION BY RADIATIVELY DRIVEN OUTFLOWS IN REDDENED QSOs","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; McGill University","funders":"California Institute of Technology; University of California, Los Angeles; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; QSOS; Star formation; Luminosity; Galaxy; Photometry (optics); Infrared; Luminous infrared galaxy; Astronomy; Quasar; Stars","score_opus":0.01924305624858365,"score_gpt":0.25910053742180383,"score_spread":0.23985748117322017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996151155","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99940133,0.000064352644,0.00013495126,0.000008376146,0.0000011961504,0.000001714204,0.00003584087,0.0000072133935,0.00034508237],"genre_scores_gemma":[0.99975485,0.000022699409,0.000069815826,0.000011412968,0.000005370117,0.0000015350776,0.0000653858,0.0000012690246,0.00006764871],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996828,0.00004717179,0.000041190135,0.00006599765,0.00008114026,0.00008169916],"domain_scores_gemma":[0.99639785,0.0008321599,0.0015556107,0.00024067026,0.0002705237,0.000703022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050925964,0.00026644635,0.00025106326,0.00083140814,0.0002851542,0.0005891496,0.00037149043,0.00042015346,0.0015349662],"category_scores_gemma":[0.0016613228,0.0001848207,0.00017707441,0.00030379108,0.00087476434,0.0003651292,0.0007251923,0.0003019002,0.00018188801],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020538637,0.000055422413,0.9284343,0.000035906876,0.00003693665,0.00052389863,0.00027579913,0.00025993076,0.06680507,0.0002460177,0.000039214192,0.0030822067],"study_design_scores_gemma":[0.0000110076835,0.00014555822,0.99517643,0.0000060404573,0.00001433772,0.0007313981,0.000096105316,0.00033118963,0.0031528657,0.00011756958,0.00021211342,0.000005403396],"about_ca_topic_score_codex":0.0007340739,"about_ca_topic_score_gemma":0.0010893029,"teacher_disagreement_score":0.0015349662,"about_ca_system_score_codex":0.00023772934,"about_ca_system_score_gemma":0.00011200776,"threshold_uncertainty_score":0.0051349998},"labels":[],"label_agreement":null},{"id":"W1996186304","doi":"10.1088/0004-637x/692/1/335","title":"<i>FAR ULTRAVIOLET SPECTROSCOPIC EXPLORER</i>OBSERVATIONS OF KPD 2055+3111, A STAR BEHIND THE CYGNUS LOOP","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Astronomy; Line (geometry); Supernova; Line-of-sight; Interstellar medium; Emission spectrum; Population; Spectral line; Galaxy","score_opus":0.015780434727867616,"score_gpt":0.23179458537873504,"score_spread":0.21601415065086743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996186304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966235,0.00006473287,0.00018730506,0.000037725527,0.0000048538086,0.0000061011524,0.0006974609,0.000041931824,0.0023362972],"genre_scores_gemma":[0.9955907,0.00004299913,0.001250873,0.00005645121,0.0000066188654,0.0000043069167,0.002321669,0.000005569786,0.00072083896],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999361,0.0000037037257,0.0000033784288,0.000013716959,0.000024923625,0.000018265111],"domain_scores_gemma":[0.9998503,0.000011536526,0.000043933764,0.000011542733,0.0000258143,0.000056735895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010838453,0.00014208013,0.0001079438,0.00048570387,0.00046959252,0.0002952573,0.00014965977,0.00017089429,0.001134999],"category_scores_gemma":[0.00015899815,0.0000735745,0.00008892748,0.00027261686,0.00010282044,0.00014616511,0.00024521534,0.00017647537,0.0002921099],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006104944,0.0002620238,0.68579054,0.00012333224,0.00010816391,0.003647597,0.0007112506,0.0013449135,0.2626416,0.00049889344,0.0032898607,0.0409712],"study_design_scores_gemma":[0.00001019779,0.00016623877,0.986188,0.000009306835,0.000016032227,0.0006976183,0.00016438133,0.0008512621,0.0074580037,0.000060019593,0.004369314,0.000009537293],"about_ca_topic_score_codex":0.0065001636,"about_ca_topic_score_gemma":0.023011398,"teacher_disagreement_score":0.0065001636,"about_ca_system_score_codex":0.00024325257,"about_ca_system_score_gemma":0.00015323226,"threshold_uncertainty_score":0.012924612},"labels":[],"label_agreement":null},{"id":"W1996260578","doi":"10.1086/589849","title":"The Impact of Halo Properties, Energy Feedback, and Projection Effects on the Mass‐SZ Flux Relation","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Chemical Physics Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Halo; Substructure; RADIUS; Cluster (spacecraft); Measure (data warehouse); Line-of-sight; Projection (relational algebra); Galaxy cluster","score_opus":0.011282264195548888,"score_gpt":0.22322002084509276,"score_spread":0.21193775664954387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996260578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931844,0.00015871356,0.005510465,0.000034558863,0.0000021579876,0.000009337387,0.00037815952,0.00009998976,0.0006223299],"genre_scores_gemma":[0.9990095,0.000027090611,0.00053827505,0.000005625725,0.00000248737,0.0000030653935,0.00033481343,0.000023391616,0.000055736393],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991555,0.0002762666,0.000055237564,0.00024491997,0.0001829558,0.000085065476],"domain_scores_gemma":[0.98737806,0.008778534,0.0015937417,0.0013562076,0.00068064744,0.00021280612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019490831,0.0006193228,0.0004984057,0.0008090093,0.0002690412,0.00090790685,0.0005018595,0.000350214,0.0009632518],"category_scores_gemma":[0.010162403,0.00037948403,0.000611456,0.00069301215,0.00061758637,0.0005904965,0.0011000072,0.00042156104,0.00022142779],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005510346,0.000040287316,0.84948874,0.00008643238,0.0006984121,0.00027002202,0.0002849657,0.11333649,0.024221936,0.0010915099,0.00023680834,0.009693437],"study_design_scores_gemma":[0.000026210691,0.00019327228,0.8577814,0.000014926884,0.00015806242,0.00033209394,0.00015914283,0.12586232,0.013917562,0.0010424444,0.00047030556,0.000042325904],"about_ca_topic_score_codex":0.003438187,"about_ca_topic_score_gemma":0.00229354,"teacher_disagreement_score":0.003438187,"about_ca_system_score_codex":0.00040139572,"about_ca_system_score_gemma":0.00020103561,"threshold_uncertainty_score":0.010307908},"labels":[],"label_agreement":null},{"id":"W1996346684","doi":"10.1088/0004-637x/762/1/31","title":"THE<sup>12</sup>C +<sup>12</sup>C REACTION AND THE IMPACT ON NUCLEOSYNTHESIS IN MASSIVE STARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Keele University; Western Canada Research Grid; Compute Canada; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Victoria; National Science Foundation","keywords":"Nucleosynthesis; Physics; Stars; Photodisintegration; r-process; s-process; Metallicity; Reaction rate; Explosive material; Nuclear reaction; Astrophysics; Isotope; Stellar nucleosynthesis; Neutron; Nuclear physics; Atomic physics; Chemistry","score_opus":0.013392471330501761,"score_gpt":0.2736304660896936,"score_spread":0.26023799475919185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996346684","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92945176,0.009212332,0.025411,0.00042263634,0.00019958027,0.000055428045,0.0024744093,0.00060619705,0.03216672],"genre_scores_gemma":[0.9924021,0.0011992436,0.002784926,0.000055708635,0.000028861708,0.000023675468,0.0009747393,0.00015826657,0.00237247],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99963665,0.00006162429,0.000022847658,0.00008437072,0.00014578842,0.00004873498],"domain_scores_gemma":[0.9993735,0.0002700213,0.00014815558,0.000073183655,0.000085259555,0.000049868955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008310367,0.0011455449,0.00037366504,0.0005091742,0.0006747179,0.0013519768,0.00076995115,0.0008376828,0.0046773073],"category_scores_gemma":[0.0015612094,0.0003089899,0.0008838308,0.00059934903,0.0005811437,0.00075395283,0.00061131525,0.00032698334,0.0013575171],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021284001,0.00017661967,0.1741019,0.0011303244,0.00035136144,0.0017270304,0.0002667482,0.6379368,0.06863273,0.04415678,0.0028052246,0.06658613],"study_design_scores_gemma":[0.000116989184,0.0006196467,0.16391635,0.00033506766,0.0004947225,0.0014088053,0.00045400453,0.615345,0.13988434,0.03745996,0.03974561,0.00021960528],"about_ca_topic_score_codex":0.0050571617,"about_ca_topic_score_gemma":0.0039422414,"teacher_disagreement_score":0.0050571617,"about_ca_system_score_codex":0.0012533511,"about_ca_system_score_gemma":0.00062510744,"threshold_uncertainty_score":0.015647113},"labels":[],"label_agreement":null},{"id":"W1996347199","doi":"10.1086/312480","title":"Statistics of Dark Matter Halos from Gravitational Lensing","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Dark matter; Weak gravitational lensing; Gravitational lens; Halo; Strong gravitational lensing; Gravitational lensing formalism; Astrophysics; Galaxy; Dark matter halo; Redshift","score_opus":0.0066778689996859555,"score_gpt":0.21072111365025703,"score_spread":0.20404324465057108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996347199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9652375,0.00020652203,0.03176453,0.000064210675,0.000005716581,0.000012814314,0.0008440446,0.00025180643,0.001612742],"genre_scores_gemma":[0.9965605,0.00009246557,0.0018962628,0.0000100361185,0.000010588291,0.000005409786,0.0012403755,0.000025187956,0.0001592473],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99961346,0.00008724155,0.00002050161,0.00007610809,0.00013557593,0.000067151705],"domain_scores_gemma":[0.9951951,0.001924336,0.0010974924,0.000751416,0.0006131501,0.00041848214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016217135,0.0004243471,0.00037307685,0.0024353063,0.0002501417,0.0012747882,0.00046899417,0.00029299772,0.00095911336],"category_scores_gemma":[0.010965999,0.00022813985,0.00029663,0.0013356253,0.0007659828,0.0010628175,0.0009747549,0.00028439888,0.00022493284],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007639278,0.000058393263,0.6143385,0.00019907793,0.00034738483,0.00036399212,0.0005849021,0.25777104,0.024640184,0.04830105,0.0016947269,0.050936844],"study_design_scores_gemma":[0.000036887825,0.00015093101,0.37798777,0.00004451656,0.000087534456,0.0004905654,0.00019373272,0.5230792,0.025369963,0.06967601,0.0027467948,0.000136096],"about_ca_topic_score_codex":0.0021543538,"about_ca_topic_score_gemma":0.0011883763,"teacher_disagreement_score":0.0024353063,"about_ca_system_score_codex":0.0006640437,"about_ca_system_score_gemma":0.0003604194,"threshold_uncertainty_score":0.008576512},"labels":[],"label_agreement":null},{"id":"W1996357848","doi":"10.1088/0004-637x/740/2/110","title":"THE FACTORY AND THE BEEHIVE. I. ROTATION PERIODS FOR LOW-MASS STARS IN PRAESEPE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Lawrence Berkeley National Laboratory; University of Oxford; National Energy Research Scientific Computing Center; Weizmann Institute of Science; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Open cluster; Angular momentum; Stellar rotation; Stars; Rotation (mathematics); Star cluster; Rotation period; Astronomy; Cluster (spacecraft); Stellar mass; Star formation; Classical mechanics","score_opus":0.014211564341805032,"score_gpt":0.22356415036654848,"score_spread":0.20935258602474344,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996357848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991309,0.000048798614,0.00008054445,0.000010685461,5.7671537e-7,0.0000017895727,0.00008680101,0.0000030900233,0.0006368292],"genre_scores_gemma":[0.99917114,0.000041133808,0.000149955,0.0000050961044,9.886044e-7,0.0000028149507,0.00025799335,0.0000020620423,0.0003689204],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998952,0.000006158062,0.0000040153873,0.000054001437,0.000015711374,0.000024822839],"domain_scores_gemma":[0.99966514,0.000055318786,0.00015211137,0.000043692453,0.000033878932,0.000049913007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001633751,0.00013173939,0.00015739092,0.0011535655,0.00072516606,0.00069132214,0.00027247006,0.0002281777,0.0012556644],"category_scores_gemma":[0.00064538163,0.00016709624,0.00019348932,0.0006419766,0.00055358745,0.00052676396,0.0009154376,0.0002352208,0.00034103307],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014676123,0.000017281447,0.9798417,0.000012801382,0.00001938138,0.00019248875,0.0015818833,0.00024696183,0.009707117,0.0003478748,0.00011586596,0.0077698273],"study_design_scores_gemma":[0.0000014967422,0.00001567471,0.9988557,0.000001193513,0.0000023880928,0.00009645832,0.00021074744,0.00008874334,0.0002620569,0.00004604295,0.0004176134,0.000001993485],"about_ca_topic_score_codex":0.010270027,"about_ca_topic_score_gemma":0.021799736,"teacher_disagreement_score":0.010270027,"about_ca_system_score_codex":0.0005568603,"about_ca_system_score_gemma":0.00018579602,"threshold_uncertainty_score":0.020420492},"labels":[],"label_agreement":null},{"id":"W1996374276","doi":"10.1086/367549","title":"Structure of the H<scp>i</scp>near the Northeast Limb of the Cygnus Loop","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Telescope; Astrophysics; Hydrogen line; Line (geometry); Kinematics; Shell (structure); Velocity dispersion; Observatory; Spectral line; Radio telescope; Dispersion (optics); Very Large Telescope; Astronomy; Geometry; Optics; Galaxy","score_opus":0.005774166800740137,"score_gpt":0.1939625449892536,"score_spread":0.18818837818851347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996374276","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994599,0.0000753867,0.0002397949,0.000055187025,0.0000014615192,0.0000058047053,0.00013900014,0.000043604145,0.0048407693],"genre_scores_gemma":[0.99896836,0.000023980198,0.00019402122,0.000015384489,0.0000035648445,0.0000041764865,0.00028111957,0.0000052107107,0.0005042708],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999523,0.0000023959003,0.0000013216132,0.000016788734,0.000014291975,0.000012889541],"domain_scores_gemma":[0.9998202,0.000014586434,0.00006329312,0.0000121618095,0.000046983674,0.000042804386],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000052817122,0.000085415384,0.00012471019,0.0006573156,0.0005129512,0.0005170078,0.00033029943,0.00020226497,0.0010231648],"category_scores_gemma":[0.00038178565,0.00013349255,0.000067988,0.00046290064,0.0006274272,0.00017257633,0.00051449,0.00019761812,0.0002986638],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043563635,0.00006584487,0.5821124,0.00010803661,0.000043079617,0.001921207,0.0016936314,0.0054890723,0.3684367,0.005369624,0.0028537826,0.031471062],"study_design_scores_gemma":[0.000010017734,0.000040528357,0.9922631,0.00000940234,0.0000063156363,0.00029560056,0.00009691431,0.0023044734,0.0027872087,0.00037911566,0.0017986856,0.000008684945],"about_ca_topic_score_codex":0.021164684,"about_ca_topic_score_gemma":0.015360926,"teacher_disagreement_score":0.021164684,"about_ca_system_score_codex":0.0007305552,"about_ca_system_score_gemma":0.0003943592,"threshold_uncertainty_score":0.042082965},"labels":[],"label_agreement":null},{"id":"W1996402016","doi":"10.1086/308590","title":"Submillimeter Observations of IC 10: The Dust Properties and Neutral Carbon Content of a Low‐Metallicity Starburst","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Metallicity; Milky Way; Submillimeter Array; Galaxy; Interstellar medium; Molecular cloud; Millimeter; Star formation","score_opus":0.0518648317790854,"score_gpt":0.2171297244848547,"score_spread":0.1652648927057693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996402016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972065,0.00005645457,0.00015091193,0.000018173227,0.0000027806122,0.000009314751,0.00065640325,0.000036784313,0.0018626483],"genre_scores_gemma":[0.9973744,0.00008369652,0.00053460896,0.000039992658,0.000012374458,0.000009940577,0.0014260658,0.0000070109654,0.0005118662],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994564,0.0000022745794,0.0000020556581,0.000017220615,0.000009949869,0.000022996748],"domain_scores_gemma":[0.99977463,0.000021059188,0.000056841538,0.00002041033,0.000021117066,0.000105931285],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099168334,0.00030901757,0.0001974343,0.00061405625,0.00030855654,0.0003512187,0.0002755204,0.00023874376,0.0011085005],"category_scores_gemma":[0.00019471136,0.00015248165,0.00013337345,0.00037586348,0.00014568756,0.0002003215,0.00034240264,0.00033974266,0.00035062592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030561106,0.00024492104,0.87242234,0.0000547299,0.000078340236,0.0005477651,0.00073314516,0.0007498451,0.10687553,0.00017713627,0.001235718,0.016574886],"study_design_scores_gemma":[0.0000061966207,0.00006646378,0.9971956,0.000003226639,0.000012339411,0.00017296999,0.000050096296,0.0002909146,0.0014489148,0.00001972769,0.00072994025,0.0000037031334],"about_ca_topic_score_codex":0.01029274,"about_ca_topic_score_gemma":0.026670031,"teacher_disagreement_score":0.01029274,"about_ca_system_score_codex":0.00039349849,"about_ca_system_score_gemma":0.00013265265,"threshold_uncertainty_score":0.020465672},"labels":[],"label_agreement":null},{"id":"W1996480473","doi":"10.1086/312585","title":"The Porous Atmosphere of η Carinae","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Atmosphere (unit); Eddington luminosity; Luminosity; Astrophysics; Physics; Limit (mathematics); Homogeneous; Radiation; Stellar atmosphere; Meteorology; Statistical physics; Optics; Mathematics; Stars","score_opus":0.006315862808768125,"score_gpt":0.20658196398299436,"score_spread":0.20026610117422625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996480473","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963091,0.0001857488,0.00086832297,0.000083505125,0.000007410957,0.0000047713947,0.00005903273,0.000016282982,0.0024658353],"genre_scores_gemma":[0.9994609,0.000095951786,0.00017780055,0.000009526026,0.000009642214,0.0000021713847,0.00004340492,0.000003973543,0.00019661478],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.00000989783,0.000002588369,0.000014111995,0.000013085162,0.00002288293],"domain_scores_gemma":[0.99975055,0.00004858409,0.00008920613,0.000021454047,0.000016455539,0.000073640374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012428472,0.00022640306,0.00019895515,0.00034003347,0.00061075325,0.0007152205,0.0003859867,0.00039858432,0.0005807741],"category_scores_gemma":[0.00066841434,0.00014825237,0.00023123313,0.00023125495,0.0008162444,0.0005526314,0.001013125,0.00038743086,0.0000721067],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066235586,0.00032283587,0.36346826,0.00029315878,0.00036472332,0.0049701408,0.002696447,0.36982468,0.085579716,0.1545497,0.0017893325,0.01547868],"study_design_scores_gemma":[0.00011683327,0.00034455548,0.5003352,0.000036632293,0.00013705855,0.0010684178,0.0020386637,0.44186556,0.0037176502,0.041534502,0.008700119,0.000104734456],"about_ca_topic_score_codex":0.006315857,"about_ca_topic_score_gemma":0.0028447367,"teacher_disagreement_score":0.006315857,"about_ca_system_score_codex":0.00044753103,"about_ca_system_score_gemma":0.00019347643,"threshold_uncertainty_score":0.012558162},"labels":[],"label_agreement":null},{"id":"W1996553064","doi":"10.1088/0004-637x/753/2/174","title":"DISCOVERY OF THE OPTICAL/ULTRAVIOLET/GAMMA-RAY COUNTERPART TO THE ECLIPSING MILLISECOND PULSAR J1816+4510","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Space Telescope Science Institute; University of Wisconsin-Milwaukee; University of Wisconsin-Madison; National Science Foundation; Yale University; National Aeronautics and Space Administration","keywords":"Millisecond pulsar; Pulsar; Ephemeris; White dwarf; Luminosity; Brightness; Neutron star; Coincidence; Pulsar planet","score_opus":0.011550519865148696,"score_gpt":0.29644927154726086,"score_spread":0.28489875168211215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996553064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99874014,0.00013947205,0.00013367535,0.000035039713,0.000012798532,0.0000042907473,0.000074582196,0.000009692696,0.0008504588],"genre_scores_gemma":[0.9979657,0.00018279284,0.0006661061,0.00007557836,0.000053047002,0.000007740381,0.00044454788,0.0000048978864,0.0005996222],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999114,0.0000060245734,0.000007821467,0.000028800461,0.000018502355,0.000027433935],"domain_scores_gemma":[0.99964786,0.000021926071,0.00015943701,0.000026225658,0.00002160307,0.00012299312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018592468,0.00020983508,0.00021183465,0.00072304445,0.0004121851,0.0007027431,0.0003789918,0.00036545884,0.0011527593],"category_scores_gemma":[0.00029543473,0.00016665676,0.00013771633,0.00042751813,0.00031097644,0.00028564237,0.0005714167,0.00025190102,0.000354883],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031854454,0.00019545859,0.746679,0.00008801157,0.000053122054,0.0053493557,0.00054733036,0.00016985768,0.21672802,0.001060097,0.000566672,0.028244516],"study_design_scores_gemma":[0.00003407635,0.000405805,0.9703314,0.000019973202,0.000042006788,0.007762516,0.00028493302,0.0003892391,0.014181998,0.000301102,0.006235195,0.000011851383],"about_ca_topic_score_codex":0.0007272613,"about_ca_topic_score_gemma":0.0012303155,"teacher_disagreement_score":0.0011527593,"about_ca_system_score_codex":0.00019545968,"about_ca_system_score_gemma":0.00010590052,"threshold_uncertainty_score":0.003856361},"labels":[],"label_agreement":null},{"id":"W1996562241","doi":"10.1086/505191","title":"Accurate Astrometry and Photometry of Saturated and Coronagraphic Point Spread Functions","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Strehl ratio; Astrometry; Photometry (optics); Point spread function; Coronagraph; Adaptive optics; Sky; High dynamic range","score_opus":0.008278477328063447,"score_gpt":0.21919754316233162,"score_spread":0.21091906583426817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996562241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.56286377,0.0007935757,0.41493982,0.00015739903,0.00008209621,0.00017314355,0.00128599,0.0040199975,0.015684213],"genre_scores_gemma":[0.79648614,0.00044444294,0.19725125,0.000069086214,0.000043502336,0.000099658886,0.0013705796,0.00070138945,0.003533947],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9992174,0.00009320517,0.000034969573,0.00019621533,0.00037764982,0.00008054949],"domain_scores_gemma":[0.99863285,0.00015530223,0.00019137621,0.00047839058,0.00041149018,0.00013048346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007804987,0.00037258462,0.00047757247,0.0013777916,0.00049361255,0.00071643613,0.00058952475,0.0005708125,0.0028439467],"category_scores_gemma":[0.0019185616,0.00028786832,0.0002951974,0.0013810575,0.00047735262,0.00094645907,0.0007783185,0.0005635112,0.0012428293],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062025926,0.00013742385,0.06333551,0.00029908784,0.000078263445,0.00023719406,0.0008056868,0.0075819083,0.66901314,0.0051788464,0.003001039,0.2497117],"study_design_scores_gemma":[0.0001141503,0.00058394065,0.47840157,0.00009945595,0.00015746117,0.0023378772,0.00038898533,0.0697822,0.40622047,0.005537963,0.036215387,0.00016060052],"about_ca_topic_score_codex":0.0017367408,"about_ca_topic_score_gemma":0.0022013288,"teacher_disagreement_score":0.0028439467,"about_ca_system_score_codex":0.0004617894,"about_ca_system_score_gemma":0.0005408154,"threshold_uncertainty_score":0.009513974},"labels":[],"label_agreement":null},{"id":"W1996563786","doi":"10.1088/0004-637x/703/2/2024","title":"THE GALAXY POPULATION OF LOW-REDSHIFT ABELL CLUSTERS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Brightest cluster galaxy; Astronomy; Galaxy cluster; Elliptical galaxy; Dwarf galaxy; Galaxy group; Population; Lenticular galaxy; Abell 2744; Interacting galaxy; Galaxy","score_opus":0.005239584369351914,"score_gpt":0.21047510486527637,"score_spread":0.20523552049592447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996563786","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993742,0.00005088366,0.00003961459,0.000011253352,6.745652e-7,0.0000020176533,0.00028267584,0.00000499054,0.00023368902],"genre_scores_gemma":[0.9981741,0.00004493393,0.00007161069,0.000016467899,0.000004541218,0.000004753296,0.0013144236,0.00000570228,0.0003635699],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962425,0.000050129445,0.000024916852,0.00010270211,0.000085072104,0.00011285076],"domain_scores_gemma":[0.99876404,0.00018862399,0.00037991445,0.00011499978,0.00018752021,0.00036494437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039044712,0.0002220716,0.0004977536,0.0019919996,0.0007839686,0.0011670347,0.00035965827,0.00020957114,0.0020414975],"category_scores_gemma":[0.0013811515,0.00015312374,0.00013008031,0.0010229094,0.00046973236,0.00037166808,0.0005889932,0.00019337315,0.0007156033],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000091786394,0.000019504916,0.9941757,0.000008917728,0.000022094884,0.00006229857,0.0003130235,0.00007628556,0.0030891707,0.00012575804,0.00018569641,0.0018297156],"study_design_scores_gemma":[0.0000023892892,0.000014782567,0.99932194,0.0000012865253,0.000005213464,0.00007721754,0.00011056948,0.00008623322,0.00015592454,0.000023861297,0.00019754631,0.0000030802887],"about_ca_topic_score_codex":0.020099554,"about_ca_topic_score_gemma":0.021107621,"teacher_disagreement_score":0.020099554,"about_ca_system_score_codex":0.00080900505,"about_ca_system_score_gemma":0.000334711,"threshold_uncertainty_score":0.039965093},"labels":[],"label_agreement":null},{"id":"W1996644459","doi":"10.1088/0004-637x/706/1/306","title":"FAR-ULTRAVIOLET DUST ALBEDO MEASUREMENTS IN THE UPPER SCORPIUS CLOUD USING THE SPINR SOUNDING ROCKET EXPERIMENT","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Sounding rocket; Albedo (alchemy); Radiative transfer; Flux (metallurgy); Geometric albedo; Spectrograph; Rocket (weapon)","score_opus":0.038661922476424165,"score_gpt":0.2769263741250579,"score_spread":0.23826445164863372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996644459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99760133,0.000020226174,0.00036246108,0.0000131535435,0.0000019219783,0.000006648883,0.00039691332,0.00009136553,0.0015060571],"genre_scores_gemma":[0.99705696,0.000030845782,0.001141022,0.000020691132,0.000004817597,0.000008127437,0.0011249579,0.000034712644,0.00057772093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983954,0.000009733672,0.0000039233564,0.00006292565,0.00005064229,0.000033136756],"domain_scores_gemma":[0.99982506,0.000024492138,0.000030231526,0.000028136987,0.000035608056,0.000056412366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024165913,0.00027966918,0.00027176517,0.0007326608,0.0005032406,0.000318904,0.00023898197,0.00018237477,0.001347846],"category_scores_gemma":[0.00026336158,0.00020424013,0.00029281425,0.00041191818,0.00026190325,0.00022801546,0.00042178793,0.00037142987,0.00023558979],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009570411,0.00030082228,0.5862594,0.00008419019,0.00020654993,0.00081541,0.0006218725,0.006402119,0.3687283,0.00046134993,0.0020018579,0.033161014],"study_design_scores_gemma":[0.000029410356,0.00007196819,0.98476356,0.0000060239613,0.000019144656,0.000111917194,0.000045100373,0.003615015,0.010576608,0.000057748326,0.0006922821,0.000011298031],"about_ca_topic_score_codex":0.02195589,"about_ca_topic_score_gemma":0.04181086,"teacher_disagreement_score":0.02195589,"about_ca_system_score_codex":0.00049995683,"about_ca_system_score_gemma":0.00019166782,"threshold_uncertainty_score":0.04365617},"labels":[],"label_agreement":null},{"id":"W1996772297","doi":"10.1086/519270","title":"Optically Thick Radio Cores of Narrow‐Waist Bipolar Nebulae","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Collimated light; Telescope; Ionization; Core (optical fiber); Radio telescope; H II region","score_opus":0.010958402659307897,"score_gpt":0.2718613612123112,"score_spread":0.2609029585530033,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996772297","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942845,0.00016866568,0.00009153591,0.0000056731888,0.0000014807783,0.000004978186,0.00004591496,0.0000026435844,0.0002507081],"genre_scores_gemma":[0.99888927,0.00014788861,0.00047078618,0.000030271514,0.000009180051,0.00000585633,0.00023256626,0.0000022570111,0.00021198454],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991524,0.0000071262357,0.0000068228314,0.000022467886,0.000018250907,0.00003009961],"domain_scores_gemma":[0.99961203,0.000040792012,0.0002016481,0.000021533471,0.000034194414,0.00008985759],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018859703,0.00022606723,0.00012430677,0.00064486515,0.00034107352,0.00048095325,0.00017626499,0.00019029735,0.0006824645],"category_scores_gemma":[0.0005184423,0.0002305929,0.00010410567,0.00024003335,0.0002508601,0.0001810217,0.00045425852,0.00014502725,0.00022212073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025140087,0.00005407584,0.8959548,0.000046431804,0.000036638427,0.0017739808,0.0005481906,0.00012200807,0.08904241,0.00015033965,0.00025715213,0.011762532],"study_design_scores_gemma":[0.000021432023,0.00020296106,0.9870228,0.000018953995,0.000032744323,0.0038079396,0.00032165437,0.00015299833,0.0063244193,0.0001437185,0.0019416435,0.00000866469],"about_ca_topic_score_codex":0.0010100299,"about_ca_topic_score_gemma":0.0017448043,"teacher_disagreement_score":0.0010100299,"about_ca_system_score_codex":0.00011597882,"about_ca_system_score_gemma":0.00009072866,"threshold_uncertainty_score":0.0022830963},"labels":[],"label_agreement":null},{"id":"W1996990230","doi":"10.1088/0004-637x/768/1/11","title":"ISOTROPIC HEATING OF GALAXY CLUSTER CORES VIA RAPIDLY REORIENTING ACTIVE GALACTIC NUCLEUS JETS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Active galactic nucleus; Supermassive black hole; Intracluster medium; Accretion (finance); Cluster (spacecraft); Quasar; Galaxy cluster; Galaxy; Astrophysical jet","score_opus":0.010054207000831357,"score_gpt":0.2277279484090245,"score_spread":0.21767374140819315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996990230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99086505,0.00033213897,0.0036568297,0.00006946101,0.00001543293,0.000009351034,0.00002570494,0.00016058097,0.0048653614],"genre_scores_gemma":[0.9992467,0.00006960255,0.00024241465,0.0000175776,0.000009267709,0.0000025683742,0.000011334609,0.000012431253,0.00038813023],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999385,0.000005107913,0.0000020269374,0.000016745777,0.0000098859355,0.000027736556],"domain_scores_gemma":[0.9998258,0.000025204394,0.000059180053,0.000039642324,0.000015099414,0.000035066398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010474765,0.00019973883,0.00021691581,0.00021183325,0.00023516653,0.0005468454,0.00036423848,0.00016190602,0.0010757754],"category_scores_gemma":[0.00035794408,0.00021755023,0.00020104306,0.00011012747,0.00031586122,0.0003046987,0.00053368724,0.00020419806,0.00030328435],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057091424,0.00011370521,0.10505863,0.00018777275,0.00013735665,0.0022607602,0.0008767202,0.08615476,0.7589934,0.012686295,0.001673139,0.031286612],"study_design_scores_gemma":[0.0002553287,0.0006904679,0.6332662,0.00004884349,0.00020157077,0.0022176784,0.00077134,0.19896829,0.1419813,0.012034643,0.009444091,0.00012020614],"about_ca_topic_score_codex":0.0019412681,"about_ca_topic_score_gemma":0.0023149643,"teacher_disagreement_score":0.0019412681,"about_ca_system_score_codex":0.00048019653,"about_ca_system_score_gemma":0.00018519854,"threshold_uncertainty_score":0.0038599372},"labels":[],"label_agreement":null},{"id":"W1996990654","doi":"10.1086/498501","title":"<i>HST</i> Imaging of MEGA Microlensing Candidates in M31","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Gravitational microlensing; Physics; Astrophysics; Supernova; Bulge; Halo; Brown dwarf; Stars; Astronomy; Galaxy; Flux (metallurgy)","score_opus":0.005593959407673049,"score_gpt":0.2138016664343654,"score_spread":0.20820770702669236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1996990654","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99915135,0.000032689546,0.00006921043,0.000012532527,3.9745947e-7,0.000002338065,0.0000720195,0.0000054778084,0.00065406127],"genre_scores_gemma":[0.9992393,0.000022900715,0.00029469153,0.0000071738714,0.0000019805643,0.000002198245,0.00026198232,0.0000018087326,0.00016792488],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999938,0.0000047966537,0.0000035285564,0.000012157073,0.000018280376,0.000023268514],"domain_scores_gemma":[0.9996455,0.00004121382,0.00012852064,0.000036721554,0.00003858345,0.00010951641],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013817342,0.00012166735,0.00008630792,0.0008998364,0.00040914913,0.00039470335,0.00015641174,0.00022363184,0.0015198643],"category_scores_gemma":[0.0004084064,0.00011012779,0.00010985959,0.00057663233,0.00014587941,0.00021222584,0.00034296027,0.00008303503,0.00035487404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024129289,0.000059034228,0.8546827,0.000033624437,0.000025378975,0.0014453399,0.0007177624,0.0011044681,0.122363225,0.0006024926,0.0008289984,0.017895594],"study_design_scores_gemma":[0.0000048242964,0.000045371253,0.99438864,0.0000030693122,0.0000059453887,0.00094353047,0.00015105415,0.00085704395,0.0029722706,0.000086581196,0.00053721847,0.000004459473],"about_ca_topic_score_codex":0.0028921678,"about_ca_topic_score_gemma":0.0082498,"teacher_disagreement_score":0.0028921678,"about_ca_system_score_codex":0.0001950133,"about_ca_system_score_gemma":0.00013188645,"threshold_uncertainty_score":0.0057507157},"labels":[],"label_agreement":null},{"id":"W1997070643","doi":"10.1088/0004-637x/711/2/764","title":"A PRECISE MASS MEASUREMENT OF THE INTERMEDIATE-MASS BINARY PULSAR PSR J1802 – 2124","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Pulsar; White dwarf; Binary pulsar; Millisecond pulsar; Pulsar planet; X-ray pulsar; Orbital period; Orbit (dynamics); Binary star","score_opus":0.013181423766039459,"score_gpt":0.2883162701060989,"score_spread":0.2751348463400594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997070643","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99391395,0.00022930071,0.0026167703,0.000030988827,0.000024430487,0.000015778653,0.000336736,0.00007165252,0.002760361],"genre_scores_gemma":[0.99638844,0.00005032393,0.002667062,0.000014750478,0.000016611413,0.000017204908,0.00042460192,0.000006406518,0.000414509],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976903,0.000033232714,0.000015327287,0.00008894673,0.000067259905,0.000026236221],"domain_scores_gemma":[0.99962926,0.000044374898,0.00015524059,0.000056641133,0.000053733533,0.000060688646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003267378,0.00026785157,0.00026776834,0.0011285137,0.00040268866,0.00039637377,0.0003296341,0.0003487856,0.0012071138],"category_scores_gemma":[0.0011786417,0.00021506422,0.00011191563,0.0006468974,0.00030002624,0.00029483286,0.00057312945,0.00029079532,0.00047770631],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054277654,0.00009283989,0.56399786,0.00008349642,0.00007537873,0.00066815974,0.0003019283,0.0005432416,0.3891582,0.0012961635,0.0008609273,0.042378996],"study_design_scores_gemma":[0.000029049721,0.0003819171,0.95803005,0.000010874162,0.00004115636,0.0015138898,0.000081200305,0.0012217211,0.03461098,0.00036277281,0.0037002137,0.0000161842],"about_ca_topic_score_codex":0.0006233348,"about_ca_topic_score_gemma":0.00094064214,"teacher_disagreement_score":0.0012071138,"about_ca_system_score_codex":0.00024797296,"about_ca_system_score_gemma":0.00015477414,"threshold_uncertainty_score":0.0040382147},"labels":[],"label_agreement":null},{"id":"W1997197659","doi":"10.1088/0004-637x/712/2/1147","title":"CAVITY OF MOLECULAR GAS ASSOCIATED WITH SUPERNOVA REMNANT 3C 397","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Supernova remnant; Physics; Molecular cloud; Astrophysics; Galactic plane; Supernova; Perpendicular; Line (geometry); Astronomy; Stars; Geometry","score_opus":0.004979075912171475,"score_gpt":0.20154463308509174,"score_spread":0.19656555717292026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997197659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99803466,0.00007757667,0.00021096418,0.00001424408,0.0000031755994,0.0000060863017,0.00015021788,0.000033122935,0.001469993],"genre_scores_gemma":[0.9991345,0.000039019866,0.00025680955,0.000008754883,0.0000042965485,0.000002603708,0.00036304965,0.0000044934054,0.00018654754],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993896,0.0000027427982,0.0000037572713,0.00001529524,0.000019089297,0.00002014986],"domain_scores_gemma":[0.9998789,0.000007722849,0.000050680424,0.000013823119,0.0000147685905,0.00003409965],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000063614214,0.00016485059,0.00018905288,0.00042212382,0.00048818535,0.00041676656,0.00030393014,0.0001753992,0.0008932328],"category_scores_gemma":[0.00014938232,0.00012926459,0.00018308495,0.00033017003,0.00030539726,0.00016945906,0.0005508948,0.0001492966,0.000213488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043802,0.00007965617,0.68268967,0.00011115818,0.00008675893,0.009291164,0.000866063,0.0011104138,0.28988716,0.0020275211,0.0010024647,0.012409934],"study_design_scores_gemma":[0.00003077867,0.00018379967,0.960505,0.000026458683,0.00005962448,0.006510236,0.0006649667,0.0030219378,0.022615856,0.00042869366,0.005927558,0.000024928511],"about_ca_topic_score_codex":0.0064272466,"about_ca_topic_score_gemma":0.0067109824,"teacher_disagreement_score":0.0064272466,"about_ca_system_score_codex":0.0003437154,"about_ca_system_score_gemma":0.00019216226,"threshold_uncertainty_score":0.012779713},"labels":[],"label_agreement":null},{"id":"W1997200226","doi":"10.1088/0004-637x/762/1/52","title":"THE DEBRIS DISK AROUND γ DORADUS RESOLVED WITH<i>HERSCHEL</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Debris; Debris disk; Luminosity; Planet; Planetary system; Dust lane; Event (particle physics)","score_opus":0.011041644931685109,"score_gpt":0.23204446127539322,"score_spread":0.2210028163437081,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997200226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994437,0.000491278,0.000195169,0.00006308474,0.00000733331,0.000004829903,0.0007673855,0.00012042834,0.0039134794],"genre_scores_gemma":[0.99782205,0.00016635354,0.0005331173,0.00003203484,0.000019317444,0.0000030183492,0.0010539003,0.00001383938,0.0003563258],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994016,0.0000058165974,0.0000020347554,0.00001624722,0.000014967926,0.00002078067],"domain_scores_gemma":[0.99986076,0.0000220861,0.00005563247,0.000022072076,0.0000136587005,0.000025654921],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008883026,0.00019914533,0.00018465704,0.00064921635,0.00032960647,0.00035488908,0.0003034955,0.0003297397,0.0010603362],"category_scores_gemma":[0.00023433259,0.00015078034,0.00014759492,0.00037295968,0.00019571443,0.00027634623,0.00028550622,0.00021748572,0.0003319995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010050961,0.0002126852,0.6829188,0.00039217036,0.0004608257,0.0031245074,0.001083096,0.011736283,0.23604622,0.0020320953,0.007712162,0.053276062],"study_design_scores_gemma":[0.000036884805,0.00008028219,0.9803305,0.000027820295,0.000053274125,0.0007982531,0.00016399604,0.004057002,0.006483736,0.000265983,0.007680548,0.000021774535],"about_ca_topic_score_codex":0.005181448,"about_ca_topic_score_gemma":0.009193341,"teacher_disagreement_score":0.005181448,"about_ca_system_score_codex":0.0004548526,"about_ca_system_score_gemma":0.00009008209,"threshold_uncertainty_score":0.010302603},"labels":[],"label_agreement":null},{"id":"W1997227664","doi":"10.1088/0004-637x/764/2/176","title":"WIDESPREAD AND HIDDEN ACTIVE GALACTIC NUCLEI IN STAR-FORMING GALAXIES AT REDSHIFT &gt;0.3","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Jet Propulsion Laboratory; National Aeronautics and Space Administration; California Institute of Technology; Smithsonian Astrophysical Observatory; Fonds Québécois de la Recherche sur la Nature et les Technologies; W. M. Keck Foundation; Smithsonian Institution; National Science Foundation","keywords":"Active galactic nucleus; Galaxy; Luminous infrared galaxy; Redshift; Infrared; Star formation; Radio galaxy","score_opus":0.007220388704389526,"score_gpt":0.20655025100089608,"score_spread":0.19932986229650657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997227664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99956065,0.00007476345,0.000036584566,0.000011567883,5.7157763e-7,0.0000011019046,0.00010784752,0.000004860338,0.00020196529],"genre_scores_gemma":[0.9996892,0.000031055784,0.00004585088,0.0000074443237,0.000002426173,7.696253e-7,0.0001577403,0.0000014678257,0.00006410689],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981123,0.000023484225,0.000012455333,0.000051304047,0.00004524191,0.000056197714],"domain_scores_gemma":[0.9988568,0.0001312991,0.00063143525,0.00006462229,0.00006348991,0.00025242515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027120917,0.00017605317,0.00016902303,0.0014300443,0.00026165316,0.00061721064,0.00031934207,0.00026160828,0.001043637],"category_scores_gemma":[0.0006693993,0.00011156582,0.00017126345,0.00097388984,0.00058121985,0.00030372475,0.0005050852,0.00023829962,0.0002811642],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033602864,0.0000113403885,0.9957332,0.000003420292,0.000009929313,0.000053592856,0.00014113673,0.00003117838,0.0022517897,0.000091216876,0.000051055336,0.0015885355],"study_design_scores_gemma":[0.0000010431114,0.0000131130355,0.99950004,8.7591854e-7,0.0000032169646,0.00013011317,0.00007194213,0.000066319764,0.000118731914,0.000029519417,0.00006419435,8.4827326e-7],"about_ca_topic_score_codex":0.0103928745,"about_ca_topic_score_gemma":0.017662432,"teacher_disagreement_score":0.0103928745,"about_ca_system_score_codex":0.00032576054,"about_ca_system_score_gemma":0.00016190171,"threshold_uncertainty_score":0.020664752},"labels":[],"label_agreement":null},{"id":"W1997262643","doi":"10.1088/0004-637x/768/2/184","title":"GALACTIC ULTRACOMPACT X-RAY BINARIES: DISK STABILITY AND EVOLUTION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"White dwarf; Instability; Accretion (finance); Dwarf nova; Cataclysmic variable star; Spectral line; Star (game theory); Stars; Helium","score_opus":0.012162210073062141,"score_gpt":0.2220192523988993,"score_spread":0.20985704232583716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997262643","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993949,0.0001326861,0.00014559408,0.000005815577,7.6990074e-7,0.0000013741951,0.000090554415,0.0000052554647,0.00022317414],"genre_scores_gemma":[0.9992293,0.00008931204,0.00027418297,0.0000053957465,0.0000041433245,0.0000020031741,0.00028061165,0.0000046119667,0.000110318564],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994135,0.0000061275846,0.0000045660795,0.000023323892,0.000010032054,0.000014639938],"domain_scores_gemma":[0.9996388,0.000054085398,0.00019284898,0.000029821716,0.00002018454,0.00006429357],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001935936,0.00031596934,0.0003003024,0.0010311096,0.00049110496,0.0010313626,0.00030494484,0.0002649207,0.00051545404],"category_scores_gemma":[0.0006545612,0.00015923378,0.00014164388,0.0010592868,0.00030499135,0.00040875224,0.0005853569,0.00025183544,0.00020250463],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013902034,0.000054765726,0.97707236,0.000023910592,0.000055208,0.00020338896,0.00018081906,0.0036028286,0.012001785,0.00041182394,0.000091954425,0.0061622844],"study_design_scores_gemma":[0.000010859967,0.0000834633,0.9704351,0.000008984034,0.000031264255,0.00037355465,0.00026361828,0.022808382,0.00476638,0.0006940146,0.0005101129,0.000014133747],"about_ca_topic_score_codex":0.004068545,"about_ca_topic_score_gemma":0.0048240824,"teacher_disagreement_score":0.004068545,"about_ca_system_score_codex":0.00046883238,"about_ca_system_score_gemma":0.0001365799,"threshold_uncertainty_score":0.008089721},"labels":[],"label_agreement":null},{"id":"W1997285098","doi":"10.1088/0004-637x/780/2/142","title":"THE SECOND-GENERATION<i>z</i>(REDSHIFT) AND EARLY UNIVERSE SPECTROMETER. I. FIRST-LIGHT OBSERVATION OF A HIGHLY LENSED LOCAL-ULIRG ANALOG AT HIGH-<i>z</i>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Redshift; Galaxy; Astrophysics; Spectrometer; Astronomy; Galactic astronomy; James Clerk Maxwell Telescope; Reionization; Submillimeter Array; Milky Way; Star formation; Optics","score_opus":0.007619447212162874,"score_gpt":0.1756259948127834,"score_spread":0.16800654760062053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997285098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81509906,0.003523814,0.08048451,0.0018321511,0.00044900077,0.0004156461,0.028525613,0.006993146,0.062677026],"genre_scores_gemma":[0.8395409,0.000834835,0.12351877,0.0013931636,0.00022434453,0.00028373682,0.015407902,0.00040479025,0.018391479],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997384,0.000019526035,0.000006220716,0.000079203244,0.000107243875,0.000049366416],"domain_scores_gemma":[0.999701,0.000024246487,0.000083603285,0.00004102021,0.000059150494,0.00009102171],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044555083,0.00032879578,0.00024720602,0.0008175503,0.00044199763,0.00045277915,0.00048762717,0.0004212712,0.0029311224],"category_scores_gemma":[0.0003189359,0.00024297534,0.00025222448,0.00047158217,0.00027829298,0.0007072948,0.00084405387,0.00060250255,0.0007613668],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005303257,0.0001401445,0.17298338,0.0003276531,0.00030272716,0.00058446423,0.00049324566,0.00057323783,0.6980218,0.00932983,0.032211076,0.08450212],"study_design_scores_gemma":[0.00017803363,0.00036103715,0.5825934,0.00006484494,0.00015488332,0.002076214,0.00019968221,0.006245318,0.21085773,0.003452365,0.19369827,0.00011818837],"about_ca_topic_score_codex":0.002191251,"about_ca_topic_score_gemma":0.0075403014,"teacher_disagreement_score":0.0029311224,"about_ca_system_score_codex":0.00054181454,"about_ca_system_score_gemma":0.00032884657,"threshold_uncertainty_score":0.00980556},"labels":[],"label_agreement":null},{"id":"W1997406936","doi":"10.1088/0004-637x/749/1/90","title":"THE ATACAMA COSMOLOGY TELESCOPE: A MEASUREMENT OF THE PRIMORDIAL POWER SPECTRUM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Spectral density; Matter power spectrum; Cosmology; Dark matter; Adiabatic process; Galaxy cluster; Observational cosmology; Galaxy; Weak gravitational lensing; Astronomy; Dark energy; Redshift; Quantum mechanics","score_opus":0.009309774187479756,"score_gpt":0.20834190854936704,"score_spread":0.1990321343618873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997406936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83534,0.0015845716,0.03502973,0.0013516732,0.00026227106,0.0002185196,0.022986613,0.0015940111,0.101632506],"genre_scores_gemma":[0.96171355,0.00036146474,0.025944134,0.00022902079,0.00015703052,0.00010646424,0.006242991,0.00023077764,0.005014531],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994854,0.0000874426,0.000010855969,0.00015851666,0.00020715522,0.000050609626],"domain_scores_gemma":[0.9989975,0.00012212688,0.00016766666,0.00022330422,0.00021265793,0.00027669774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009330533,0.00021505274,0.00020604827,0.0013483057,0.00072818814,0.00083044934,0.00049826386,0.0005393532,0.0031570976],"category_scores_gemma":[0.0017643791,0.00022819186,0.00024435532,0.0018159361,0.00045584832,0.00079533836,0.00086655834,0.00061117514,0.0008712959],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072481646,0.00024708404,0.6294203,0.0002915785,0.00042412852,0.00033485732,0.0022373663,0.0019183292,0.14371455,0.027738834,0.038938593,0.15400955],"study_design_scores_gemma":[0.000089273,0.000071365015,0.9453763,0.000028172633,0.000057736248,0.00028856288,0.00023431085,0.003680654,0.0064621093,0.0037189,0.03994783,0.000044852226],"about_ca_topic_score_codex":0.011551113,"about_ca_topic_score_gemma":0.019071527,"teacher_disagreement_score":0.011551113,"about_ca_system_score_codex":0.00067395606,"about_ca_system_score_gemma":0.00076658715,"threshold_uncertainty_score":0.022967756},"labels":[],"label_agreement":null},{"id":"W1997408057","doi":"10.1088/0004-637x/763/1/33","title":"SEARCHES FOR HIGH-ENERGY NEUTRINO EMISSION IN THE GALAXY WITH THE COMBINED ICECUBE-AMANDA DETECTOR","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Marsden Fund; Japan Society for the Promotion of Science; Helmholtz Alliance for Astroparticle Physics; Vetenskapsrådet; Fonds Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; Belgian Federal Science Policy Office; Bundesministerium für Bildung und Forschung; Office of Polar Programs; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Knut och Alice Wallenbergs Stiftelse; University of Oxford; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Neutrino; Galactic plane; Neutrino detector; Neutrino astronomy; Astrophysics; Galaxy; Sky; Detector; Astronomy; Telescope; Point source; Neutrino oscillation; Particle physics; Optics","score_opus":0.0090884789489608,"score_gpt":0.20950450719780836,"score_spread":0.20041602824884755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997408057","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9621788,0.002038167,0.012160358,0.00014083605,0.000043843866,0.00014403708,0.0078120087,0.0007158817,0.014766088],"genre_scores_gemma":[0.89262134,0.0010034378,0.07956445,0.00011666649,0.00011018459,0.00035178423,0.023719609,0.00014337733,0.0023692404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99930894,0.00018893112,0.00001908808,0.00016385061,0.0002141746,0.00010503703],"domain_scores_gemma":[0.99931514,0.00023105019,0.0001278887,0.00013129922,0.00011136018,0.000083224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009962389,0.00082954066,0.0007934334,0.0020061133,0.00041545476,0.000987194,0.0008609839,0.0004539235,0.0018251367],"category_scores_gemma":[0.0010512883,0.00044107882,0.0006807499,0.0020551777,0.00033343956,0.00059409166,0.0009590006,0.0003577462,0.00050904416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.006505902,0.0008961156,0.66348374,0.00059208105,0.0023517692,0.0021496993,0.0005280531,0.039616294,0.14426042,0.0061967806,0.01268128,0.120737955],"study_design_scores_gemma":[0.0010379226,0.002500276,0.6316311,0.00022568797,0.0011911559,0.005546205,0.00038171388,0.1406398,0.122716576,0.006702262,0.08708515,0.0003422098],"about_ca_topic_score_codex":0.002963829,"about_ca_topic_score_gemma":0.0067405505,"teacher_disagreement_score":0.002963829,"about_ca_system_score_codex":0.00044923043,"about_ca_system_score_gemma":0.00047190773,"threshold_uncertainty_score":0.0061056614},"labels":[],"label_agreement":null},{"id":"W1997440226","doi":"10.1086/511409","title":"A Gravito‐electrostatic Sheath Model for Surface Origin of Subsonic Solar Wind Plasma","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Solar wind; Plasma; Heliosphere; Mach number; Classical mechanics; Mechanics","score_opus":0.0114769810126883,"score_gpt":0.257050843791876,"score_spread":0.2455738627791877,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997440226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6924598,0.0017488014,0.22598362,0.0018783142,0.00019259716,0.000100442405,0.00039530112,0.00041577982,0.076825336],"genre_scores_gemma":[0.9833754,0.00044088296,0.004122181,0.00012234894,0.000059775062,0.00008364458,0.00010882147,0.00003925206,0.011647667],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999416,0.000013392049,0.0000017562626,0.000010886953,0.000015426273,0.000016954731],"domain_scores_gemma":[0.9999398,0.000010815209,0.000013034713,0.0000055669057,0.0000127603225,0.000018106315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109873945,0.00039929667,0.0003457753,0.0003355879,0.0004459673,0.0006199669,0.0010421011,0.001059084,0.0017732558],"category_scores_gemma":[0.0002858208,0.00017577842,0.000615887,0.0002759697,0.00063415564,0.0007973816,0.0007174573,0.00042749528,0.0004155023],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000895928,0.000045829536,0.0015958727,0.00006292937,0.000028928645,0.0008734026,0.00034608284,0.6158529,0.019927587,0.35578573,0.0019492762,0.0034419012],"study_design_scores_gemma":[0.00003105285,0.000046256304,0.0006522553,0.0000045926126,0.000006440762,0.00013748517,0.000055199067,0.9649097,0.00035720624,0.032289237,0.0014957365,0.000014911901],"about_ca_topic_score_codex":0.004291312,"about_ca_topic_score_gemma":0.0012480862,"teacher_disagreement_score":0.004291312,"about_ca_system_score_codex":0.0006556516,"about_ca_system_score_gemma":0.000467143,"threshold_uncertainty_score":0.008532703},"labels":[],"label_agreement":null},{"id":"W1997519655","doi":"10.1088/0004-637x/775/2/126","title":"LoCuSS: THE STEADY DECLINE AND SLOW QUENCHING OF STAR FORMATION IN CLUSTER GALAXIES OVER THE LAST FOUR BILLION YEARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Galaxy cluster; Star formation; Cluster (spacecraft); Brightest cluster galaxy; Galaxy; Accretion (finance); Galaxy group; Galaxy formation and evolution; Elliptical galaxy","score_opus":0.0078497903753356,"score_gpt":0.20715180142533957,"score_spread":0.19930201105000397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997519655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99884206,0.00013494097,0.00007155645,0.000016198252,0.0000012168459,0.0000020280775,0.00063076423,0.000016071845,0.00028533678],"genre_scores_gemma":[0.9988061,0.000058892354,0.000075813885,0.0000070595147,0.0000043606788,0.0000016490344,0.00090033194,0.0000029991866,0.0001427387],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985206,0.000017149583,0.000009670683,0.000052882853,0.000035448516,0.00003277211],"domain_scores_gemma":[0.998749,0.000109516644,0.00065417675,0.00012602392,0.000110375695,0.00025078293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033205742,0.00013623507,0.00017660245,0.0014900493,0.00018498325,0.00049349584,0.0002418359,0.00017387525,0.00079165975],"category_scores_gemma":[0.0011393771,0.00008991508,0.00023791526,0.0010396591,0.00034111564,0.00036175037,0.00052525534,0.00012156333,0.00022366745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006039431,0.000005798028,0.9939144,0.000009896338,0.000043730077,0.000036887475,0.00020755727,0.00020403853,0.0013499494,0.00007891972,0.00016788363,0.003920507],"study_design_scores_gemma":[5.721733e-7,0.000012477995,0.9995797,6.955964e-7,0.0000036549184,0.000032908076,0.00003026186,0.000099105564,0.00007552429,0.000014138828,0.0001499182,0.000001009024],"about_ca_topic_score_codex":0.008440613,"about_ca_topic_score_gemma":0.010566305,"teacher_disagreement_score":0.008440613,"about_ca_system_score_codex":0.0003122923,"about_ca_system_score_gemma":0.00014711986,"threshold_uncertainty_score":0.01678294},"labels":[],"label_agreement":null},{"id":"W1997538404","doi":"10.1088/0004-637x/738/1/56","title":"THE NATURE OF STAR FORMATION AT 24 μm IN THE GROUP ENVIRONMENT AT 0.3 ≲<i>z</i>≲ 0.55","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McMaster University; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Star formation; Galaxy; Galaxy group; Redshift; Stars; Stellar mass; Galaxy cluster; Group (periodic table); Galaxy formation and evolution; Cluster (spacecraft); Astronomy","score_opus":0.0073053599840613445,"score_gpt":0.1819621329838756,"score_spread":0.17465677299981425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997538404","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990402,0.000053499036,0.000052756583,0.000012342704,7.4853256e-7,0.0000014874057,0.0001079954,0.000004974297,0.0007260432],"genre_scores_gemma":[0.9996081,0.000022271597,0.000055092358,0.000008062309,0.0000023830478,0.0000014245198,0.00017484454,0.000002510197,0.00012522595],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998821,0.000007920054,0.000003987873,0.000035220804,0.000020322825,0.000050467595],"domain_scores_gemma":[0.9995314,0.00003855234,0.00017762666,0.00003402563,0.0000443182,0.00017410103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017355522,0.00010762744,0.00020459622,0.0008472953,0.00035563167,0.0006896914,0.00025095243,0.00017709636,0.0008417588],"category_scores_gemma":[0.0005109851,0.00013467712,0.00020016266,0.0005028229,0.0003733533,0.00028459716,0.00042704016,0.00020917707,0.00020964429],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013447402,0.000035026424,0.9762281,0.000013534213,0.00004075734,0.00009778156,0.00043437566,0.00019034123,0.018421238,0.00036805723,0.0002075353,0.0038287758],"study_design_scores_gemma":[0.0000012272391,0.000009741003,0.9994747,8.249263e-7,0.000004237176,0.00002088077,0.00006288488,0.00006825867,0.0002159532,0.000035484445,0.00010453297,0.0000013372775],"about_ca_topic_score_codex":0.012752642,"about_ca_topic_score_gemma":0.014686586,"teacher_disagreement_score":0.012752642,"about_ca_system_score_codex":0.0005576892,"about_ca_system_score_gemma":0.00014363561,"threshold_uncertainty_score":0.02535683},"labels":[],"label_agreement":null},{"id":"W1997587116","doi":"10.1088/0004-637x/706/2/l275","title":"VERITAS UPPER LIMIT ON THE VERY HIGH ENERGY EMISSION FROM THE RADIO GALAXY NGC 1275","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Fermi Gamma-ray Space Telescope; Spitzer Space Telescope; Galaxy; Crab Nebula; Radio galaxy; Astronomy; Active galactic nucleus; Telescope; Gamma ray; Flux (metallurgy); High energy","score_opus":0.007318739239878318,"score_gpt":0.19467366633208713,"score_spread":0.1873549270922088,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997587116","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8873306,0.009204326,0.025455657,0.0010527691,0.000206961,0.00003915524,0.003901613,0.0014221054,0.0713867],"genre_scores_gemma":[0.9883596,0.0008563397,0.0041972836,0.00039093764,0.00013283249,0.000027633456,0.0034625414,0.00006895966,0.0025038936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99851865,0.0001430418,0.00006345953,0.00039138604,0.0005411154,0.00034237586],"domain_scores_gemma":[0.9941453,0.002659127,0.0011683117,0.0008944934,0.00072602124,0.00040676846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018045323,0.000589604,0.0005671084,0.0021909298,0.0006213215,0.0014253571,0.0013606857,0.0008919355,0.011866655],"category_scores_gemma":[0.0037178032,0.00037169908,0.00071809854,0.00048198408,0.00084367587,0.0008167839,0.001969191,0.0008964703,0.0023110986],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0043476177,0.00030588504,0.50978327,0.0010271025,0.0009833786,0.0035055652,0.0013534371,0.010914806,0.20937583,0.07961374,0.019246247,0.15954316],"study_design_scores_gemma":[0.00020681854,0.0010497905,0.7133357,0.00078826596,0.0005469427,0.004488833,0.0005473051,0.020054445,0.11428567,0.027720619,0.11677438,0.00020122406],"about_ca_topic_score_codex":0.0062225778,"about_ca_topic_score_gemma":0.004151427,"teacher_disagreement_score":0.011866655,"about_ca_system_score_codex":0.000993289,"about_ca_system_score_gemma":0.00036699921,"threshold_uncertainty_score":0.039697945},"labels":[],"label_agreement":null},{"id":"W1997617110","doi":"10.1086/317187","title":"Simulation of Primordial Object Formation","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Western University","funders":"","keywords":"Redshift; Dark matter; Star formation; Smoothed-particle hydrodynamics; Molecular cloud; Baryon; Solar mass; Cosmology; Solar System","score_opus":0.010080564805060109,"score_gpt":0.2475737050618535,"score_spread":0.23749314025679338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997617110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9617604,0.00013319917,0.01952705,0.00035532413,0.0000841715,0.00011100196,0.0022045786,0.000748835,0.015075446],"genre_scores_gemma":[0.98144,0.000085888176,0.014326003,0.000106709376,0.000015779235,0.000115955285,0.0015948057,0.00008135941,0.002233477],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979836,0.000055887005,0.000010078852,0.00004420562,0.000039602244,0.000051904964],"domain_scores_gemma":[0.99886656,0.0005972788,0.00009303917,0.00009363242,0.00015559285,0.0001939171],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050328305,0.00044449812,0.0005724519,0.00038770484,0.0006327321,0.0007356994,0.0013642379,0.0012907555,0.0050369883],"category_scores_gemma":[0.002364209,0.00036471576,0.0005697202,0.00067729654,0.0008916499,0.00069293415,0.0009661208,0.001013083,0.00033648624],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018682785,0.00010781926,0.007187427,0.000049240913,0.000052631265,0.00015560006,0.00010396839,0.9827755,0.0012369276,0.00512504,0.0006919081,0.0023271888],"study_design_scores_gemma":[0.000075910684,0.000033676613,0.0015819991,0.0000033919728,0.000010379535,0.000015427604,0.000025393838,0.995867,0.0006140837,0.0010706668,0.0006935864,0.000008425668],"about_ca_topic_score_codex":0.029073905,"about_ca_topic_score_gemma":0.015670627,"teacher_disagreement_score":0.029073905,"about_ca_system_score_codex":0.001226816,"about_ca_system_score_gemma":0.0011865422,"threshold_uncertainty_score":0.057809353},"labels":[],"label_agreement":null},{"id":"W1997653229","doi":"10.1086/341795","title":"Seismic Test of Solar Models, Solar Neutrinos, and Implications for Metal‐rich Accretion","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Helioseismology; Standard solar model; Solar core; Convection zone; Astrophysics; Solar neutrino; Physics; Metallicity; Neutrino; Solar neutrino problem; Accretion (finance); Astronomy; Geophysics; Neutrino oscillation; Stars","score_opus":0.03544178521715688,"score_gpt":0.28228286789238144,"score_spread":0.24684108267522456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997653229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96902776,0.00037088429,0.0020309733,0.0013822991,0.000045516877,0.000011015106,0.00013917475,0.000053118183,0.026939314],"genre_scores_gemma":[0.9990953,0.00008131127,0.00029103388,0.00005510281,0.000024912173,0.0000027080293,0.00006678501,0.0000072648463,0.00037558703],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99972075,0.00011644039,0.00001639787,0.00005140396,0.000058283105,0.00003666871],"domain_scores_gemma":[0.9967049,0.0017744366,0.00064701965,0.00035280353,0.00027452924,0.00024620473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001669925,0.00032670292,0.00028264456,0.00043248737,0.0006370819,0.0018862403,0.0006528352,0.0006835053,0.0029856453],"category_scores_gemma":[0.0084062815,0.00012757037,0.0003328406,0.00046071105,0.0010752811,0.0011273699,0.00093065476,0.00039989702,0.000284336],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0032129216,0.00045439595,0.58298635,0.0002935917,0.00027719812,0.0019386765,0.0023556314,0.04602361,0.014758403,0.28549725,0.0049772053,0.057224844],"study_design_scores_gemma":[0.00055357075,0.00075401954,0.34095696,0.00016389164,0.00019866817,0.00087932317,0.0047968365,0.23405734,0.010949534,0.3968998,0.009699771,0.00009031324],"about_ca_topic_score_codex":0.0019998539,"about_ca_topic_score_gemma":0.0010087813,"teacher_disagreement_score":0.0029856453,"about_ca_system_score_codex":0.00055856886,"about_ca_system_score_gemma":0.00038547866,"threshold_uncertainty_score":0.00998801},"labels":[],"label_agreement":null},{"id":"W1997678212","doi":"10.1088/0004-637x/771/2/81","title":"HYBRID COSMOLOGICAL SIMULATIONS WITH STREAM VELOCITIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Halo; Dark matter; Accretion (finance); Smoothed-particle hydrodynamics; Redshift; Structure formation; Epoch (astronomy); Stars","score_opus":0.00821280369479717,"score_gpt":0.2035486566393837,"score_spread":0.19533585294458652,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997678212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87470555,0.0003519114,0.08801768,0.00083821215,0.00023170281,0.00018854863,0.0049572666,0.002483068,0.028226083],"genre_scores_gemma":[0.9193526,0.00020074759,0.071655326,0.0003249068,0.000063649866,0.00033510395,0.0031416793,0.0004829611,0.0044429894],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981886,0.000060406277,0.0000098033215,0.00003552745,0.000038273254,0.00003714102],"domain_scores_gemma":[0.9985372,0.0008875046,0.00011990514,0.00009619885,0.00021637086,0.00014288629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006015707,0.0005410379,0.00060676463,0.0007341642,0.00052580156,0.0010011742,0.0016221467,0.0012973333,0.0043078656],"category_scores_gemma":[0.003821469,0.00044459582,0.00077165343,0.0009422505,0.00052679185,0.0007518428,0.00095020473,0.0009246336,0.00041471346],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014418032,0.000095759446,0.004506254,0.000047479196,0.00006568758,0.000081008046,0.000097047836,0.9820494,0.0009489923,0.007856529,0.0011260732,0.0029815314],"study_design_scores_gemma":[0.00004347245,0.000011645625,0.00033834446,0.0000036472422,0.0000064713095,0.0000060293073,0.000014834478,0.99756974,0.00020827669,0.001289497,0.0005012066,0.0000067739434],"about_ca_topic_score_codex":0.028749282,"about_ca_topic_score_gemma":0.019494796,"teacher_disagreement_score":0.028749282,"about_ca_system_score_codex":0.0010735436,"about_ca_system_score_gemma":0.00109987,"threshold_uncertainty_score":0.057163894},"labels":[],"label_agreement":null},{"id":"W1997700621","doi":"10.1086/521041","title":"Modeling Lyman Continuum Emission from Young Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy; Astronomy; Star formation; Luminous infrared galaxy; Galaxy formation and evolution","score_opus":0.008483547696096683,"score_gpt":0.21928898701940025,"score_spread":0.21080543932330356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997700621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98966026,0.000114623814,0.007408014,0.00013713639,0.000010608853,0.00003073265,0.0005768891,0.00011355732,0.0019481922],"genre_scores_gemma":[0.9926267,0.00015845223,0.0045616687,0.00007075563,0.000016424254,0.000048229067,0.000689466,0.000048217524,0.0017799954],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998741,0.000038890874,0.000004953685,0.000035731933,0.000016527738,0.000029640163],"domain_scores_gemma":[0.99930584,0.00021757926,0.00018875602,0.000048979873,0.00006604333,0.00017276913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059841777,0.00058488676,0.0005497144,0.0006759282,0.0005527165,0.0010252094,0.0018623183,0.0012386102,0.0015153115],"category_scores_gemma":[0.0018605544,0.00045918577,0.0007697667,0.00088116067,0.0006162963,0.0009782764,0.0006522198,0.0008651282,0.00030921033],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015760268,0.00015042684,0.056587435,0.000031530068,0.00009132824,0.00023313945,0.00027286986,0.92969376,0.0026776055,0.007251504,0.00048582512,0.002366993],"study_design_scores_gemma":[0.000085515734,0.000053379306,0.008197565,0.0000060437983,0.00003149211,0.000055489767,0.000053158023,0.9884588,0.00041490595,0.0019624748,0.00065833196,0.00002282588],"about_ca_topic_score_codex":0.03546567,"about_ca_topic_score_gemma":0.01903604,"teacher_disagreement_score":0.03546567,"about_ca_system_score_codex":0.0017890672,"about_ca_system_score_gemma":0.0006281892,"threshold_uncertainty_score":0.070518434},"labels":[],"label_agreement":null},{"id":"W1997923796","doi":"10.1086/320969","title":"A Revised Cepheid Distance to NGC 4258 and a Test of the Distance Scale","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Cepheid variable; Cosmic distance ladder; Distance modulus; Large Magellanic Cloud; Galaxy; Metallicity; Astrometry; Hubble's law; Length scale","score_opus":0.004897612483306202,"score_gpt":0.201350290259536,"score_spread":0.1964526777762298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997923796","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.944413,0.0006556563,0.01353773,0.00043776908,0.00011654092,0.0000743458,0.001746734,0.00014825343,0.038870048],"genre_scores_gemma":[0.9902969,0.00014096648,0.0070453375,0.00008344671,0.000035100413,0.000029807574,0.0010123216,0.000054181146,0.001302052],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983046,0.00030688595,0.00009507944,0.0005273652,0.0006643248,0.00010177379],"domain_scores_gemma":[0.9965109,0.0007258421,0.0006475622,0.0009899414,0.0008413979,0.0002842826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011702189,0.00040008823,0.00023333043,0.0011301963,0.0007652843,0.0010013918,0.0011130064,0.0003826576,0.0042338343],"category_scores_gemma":[0.011075382,0.00015118862,0.00019350741,0.0013741376,0.00080130703,0.0015174058,0.0016883429,0.00075802754,0.0010108178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068916514,0.00017772903,0.68891066,0.00037934442,0.00024053322,0.0015802446,0.0052478192,0.00697093,0.030183079,0.083598174,0.010485815,0.17153649],"study_design_scores_gemma":[0.00005981087,0.00030618886,0.9457172,0.00004844574,0.000057917357,0.00080986443,0.0013540385,0.009422853,0.0038600564,0.009958041,0.028330125,0.000075534874],"about_ca_topic_score_codex":0.0070259864,"about_ca_topic_score_gemma":0.006432453,"teacher_disagreement_score":0.0070259864,"about_ca_system_score_codex":0.0007052144,"about_ca_system_score_gemma":0.0003330053,"threshold_uncertainty_score":0.014163613},"labels":[],"label_agreement":null},{"id":"W1997927321","doi":"10.1086/308623","title":"A Stationary Core with a One‐sided Jet in the Center of M81","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Very-long-baseline interferometry; Jet (fluid); Rotation (mathematics); Galactic Center; Position angle; Astronomy; Sky; Spiral galaxy; Epoch (astronomy); Core (optical fiber); Geometry; Optics","score_opus":0.01512568231891957,"score_gpt":0.23222499589759624,"score_spread":0.21709931357867668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997927321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99854976,0.000114838884,0.00020112035,0.000024467896,0.0000052905643,0.000005658452,0.000056726596,0.000015414527,0.001026783],"genre_scores_gemma":[0.99927443,0.00004207039,0.0002342306,0.000022378603,0.00001248567,0.000002931056,0.00010776637,0.0000035071919,0.00030024792],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999287,0.0000043671703,0.000008531689,0.000023593553,0.000013607205,0.000021170292],"domain_scores_gemma":[0.9996345,0.00003309024,0.00015945315,0.000058298923,0.000038400438,0.00007632819],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021570844,0.0002306417,0.00025606257,0.0005577304,0.000605655,0.00068797736,0.0003309806,0.0003850851,0.001168596],"category_scores_gemma":[0.0004976438,0.00021192232,0.00018633518,0.0004533233,0.00038154173,0.00029304466,0.00072709634,0.0001927377,0.00052242],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014404826,0.00040570466,0.771456,0.00011567788,0.00010129867,0.025267603,0.002470048,0.0013932633,0.15697435,0.0015171025,0.0014669113,0.037391562],"study_design_scores_gemma":[0.00004991514,0.00034679082,0.9880712,0.000017029919,0.000029283632,0.0049268827,0.0001980214,0.0007048941,0.0031485783,0.00024648206,0.0022489657,0.000012056618],"about_ca_topic_score_codex":0.0022295837,"about_ca_topic_score_gemma":0.0021910174,"teacher_disagreement_score":0.0022295837,"about_ca_system_score_codex":0.00036358734,"about_ca_system_score_gemma":0.00016845668,"threshold_uncertainty_score":0.0044332147},"labels":[],"label_agreement":null},{"id":"W1997943693","doi":"10.1088/0004-637x/796/2/127","title":"A DEEP<i>SPITZER</i>SURVEY OF CIRCUMSTELLAR DISKS IN THE YOUNG DOUBLE CLUSTER, h AND χ PERSEI","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Toronto","funders":"","keywords":"Stars; Photometry (optics); Spectral energy distribution; Circumstellar disk; Infrared excess; Infrared; Circumstellar dust; Photometer; Spectroscopy","score_opus":0.014937439121500312,"score_gpt":0.24477642106494948,"score_spread":0.22983898194344918,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1997943693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99945337,0.00001922696,0.00010927077,0.0000047450485,3.9433894e-7,0.0000024856336,0.00019835844,0.000008391134,0.00020384487],"genre_scores_gemma":[0.99804616,0.000025555639,0.0005549106,0.000005829142,0.0000022519039,0.000004070565,0.0011302971,0.0000026665039,0.00022834781],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999527,0.000004576193,0.0000023419407,0.000018304161,0.000009586044,0.000012509237],"domain_scores_gemma":[0.99974936,0.000022164342,0.00009717135,0.000027261101,0.000022904649,0.000081161226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011711785,0.00019514498,0.000119191,0.00083938235,0.00017858384,0.00021105121,0.00018583838,0.00011118211,0.0005388126],"category_scores_gemma":[0.0002721092,0.00009112178,0.00012710775,0.00043038328,0.00014043592,0.00014220171,0.00026523636,0.00008140839,0.00017993756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040667404,0.000027618502,0.98648703,0.000007985047,0.000028897055,0.00013851974,0.00011963683,0.001684816,0.005488048,0.00011665488,0.00028386866,0.0055763866],"study_design_scores_gemma":[0.0000028714742,0.000027247712,0.9972734,0.0000012073577,0.0000069263037,0.00009026038,0.0000635761,0.0015937543,0.00044583977,0.000054515822,0.00043796678,0.000002333194],"about_ca_topic_score_codex":0.005983035,"about_ca_topic_score_gemma":0.011435409,"teacher_disagreement_score":0.005983035,"about_ca_system_score_codex":0.00024990735,"about_ca_system_score_gemma":0.00017368354,"threshold_uncertainty_score":0.011896372},"labels":[],"label_agreement":null},{"id":"W1998145401","doi":"10.1086/504421","title":"Millimeter Observation of the SZ Effect in the Corona Borealis Supercluster","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Cosmic microwave background; Observatory; Supercluster (genetic); Planck; Physics; Sky; Astrophysics; Anisotropy; Astronomy; Millimeter; Angular resolution (graph drawing); Declination; Optics","score_opus":0.007934156384547246,"score_gpt":0.21095764088288396,"score_spread":0.2030234844983367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998145401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990158,0.000092133654,0.00020120961,0.000016849195,0.0000032779612,0.0000026269672,0.00011322317,0.000028854083,0.0005260036],"genre_scores_gemma":[0.9995753,0.000023305105,0.00021006423,0.000005392321,0.000005909742,0.0000011582861,0.00011921856,0.000003357441,0.000056222616],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99990046,0.0000119337155,0.0000035165451,0.00002889167,0.000026422098,0.000028661721],"domain_scores_gemma":[0.99974436,0.000029484087,0.00010775671,0.000035303317,0.000027553415,0.000055636498],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001260057,0.00016045506,0.00022232837,0.00031141436,0.0001790809,0.00022730653,0.00018408465,0.00011128128,0.00038076122],"category_scores_gemma":[0.00033117126,0.00010892683,0.00014866912,0.00032436536,0.00017247122,0.00010770321,0.00040048067,0.00018143402,0.00006925736],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010657859,0.00009398932,0.40655422,0.000059636175,0.00020363014,0.0007232316,0.00053976,0.0012579699,0.5741378,0.00033030094,0.0005517026,0.014481951],"study_design_scores_gemma":[0.000014319976,0.00008949635,0.992878,0.000001790136,0.000026669299,0.00022299755,0.000045946577,0.0005885774,0.0056026117,0.00003495148,0.0004889125,0.0000056511726],"about_ca_topic_score_codex":0.0026206807,"about_ca_topic_score_gemma":0.0033879008,"teacher_disagreement_score":0.0026206807,"about_ca_system_score_codex":0.00022149389,"about_ca_system_score_gemma":0.000072683215,"threshold_uncertainty_score":0.0052108765},"labels":[],"label_agreement":null},{"id":"W1998288650","doi":"10.1088/0004-637x/756/2/139","title":"EXPLORING THE DIVERSITY OF GROUPS AT 0.1 &lt;<i>z</i>&lt; 0.8 WITH X-RAY AND OPTICALLY SELECTED SAMPLES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; McMaster University","funders":"Science and Technology Facilities Council","keywords":"Velocity dispersion; Galaxy; Redshift; Stars; RADIUS; Scaling; Stellar population; Population","score_opus":0.021226948005310584,"score_gpt":0.19027535470264112,"score_spread":0.16904840669733054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998288650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952066,0.00001313749,0.00008688814,0.0000075910643,2.6369403e-7,0.0000028288578,0.000087129934,0.000003838938,0.00027770706],"genre_scores_gemma":[0.99929523,0.000008034988,0.00017080286,0.0000033520473,0.0000016466305,0.0000044493554,0.00038341174,0.000003041892,0.00013013267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997447,0.000036064812,0.000015968948,0.00007415666,0.000053125408,0.00007597797],"domain_scores_gemma":[0.9990299,0.00019744468,0.00033281147,0.000111155256,0.00012358814,0.00020499618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044742503,0.00018815017,0.00024742316,0.0020670423,0.00034643093,0.0007374693,0.00027152197,0.0002197442,0.0012673917],"category_scores_gemma":[0.000981544,0.00011349165,0.00018735083,0.0008552696,0.00039561157,0.0004051346,0.00093306927,0.0001859284,0.00032651605],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023640651,0.000057488378,0.97871566,0.000013271444,0.000039464336,0.00009161053,0.0011002015,0.00047698873,0.0111591965,0.00023735577,0.00018545288,0.007686921],"study_design_scores_gemma":[0.0000051184566,0.000048501144,0.99774206,0.0000017260176,0.000010869255,0.000060593255,0.00029586765,0.0006940102,0.0008066871,0.00006514497,0.00026675733,0.0000025327324],"about_ca_topic_score_codex":0.0027936725,"about_ca_topic_score_gemma":0.0031426656,"teacher_disagreement_score":0.0027936725,"about_ca_system_score_codex":0.00022406444,"about_ca_system_score_gemma":0.00008837697,"threshold_uncertainty_score":0.0055547953},"labels":[],"label_agreement":null},{"id":"W1998308462","doi":"10.1088/0004-637x/768/2/156","title":"INTERIOR STRUCTURE OF WATER PLANETS: IMPLICATIONS FOR THEIR DYNAMO SOURCE REGIONS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Dynamo; Planet; Exoplanet; Parameter space; Dynamo theory; Terrestrial planet; Envelope (radar); Planetary mass; Magnetic field","score_opus":0.007468070796279766,"score_gpt":0.20651153977601305,"score_spread":0.1990434689797333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998308462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99622214,0.00011086887,0.0014977707,0.000055884742,0.00000106336,0.0000063084085,0.00019845371,0.000017446404,0.0018900644],"genre_scores_gemma":[0.99902713,0.000065543405,0.00071708986,0.0000042354195,0.0000013872125,0.0000035551404,0.000086113294,0.000009980817,0.000084968924],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999529,0.000009482266,0.0000025268384,0.000015855143,0.0000074821,0.000011752454],"domain_scores_gemma":[0.99974126,0.00007486529,0.00008818881,0.000027786069,0.00001860749,0.000049288516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010812748,0.00019358438,0.0002711554,0.00041585517,0.000303754,0.0007891008,0.00022990048,0.00029429057,0.0011339913],"category_scores_gemma":[0.0008951933,0.0002770926,0.0002765845,0.00027785765,0.0005036881,0.00074048096,0.0005271562,0.00017508256,0.000114564085],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048357708,0.000070726026,0.5137407,0.00017492493,0.000103243714,0.00057922734,0.000681967,0.35628995,0.09462683,0.01651432,0.00041490092,0.016319584],"study_design_scores_gemma":[0.0001467589,0.0001223182,0.33016932,0.000052068295,0.000068710295,0.0005664168,0.00085519213,0.62665707,0.009009813,0.029280942,0.0030189746,0.000052382024],"about_ca_topic_score_codex":0.002812277,"about_ca_topic_score_gemma":0.0021790557,"teacher_disagreement_score":0.002812277,"about_ca_system_score_codex":0.0005264675,"about_ca_system_score_gemma":0.0001787288,"threshold_uncertainty_score":0.0055918097},"labels":[],"label_agreement":null},{"id":"W1998475147","doi":"10.1088/0004-637x/798/1/38","title":"AN OPTICALLY OBSCURED AGN IN A LOW MASS, IRREGULAR DWARF GALAXY: A MULTI-WAVELENGTH ANALYSIS OF J1329+3234","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supermassive black hole; Dwarf galaxy; Galaxy; Black hole (networking); Luminosity; Intermediate-mass black hole; Stellar black hole; Binary black hole","score_opus":0.011553318006145268,"score_gpt":0.24130546543824402,"score_spread":0.22975214743209876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998475147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99967134,0.00001948594,0.000041194886,0.000006310077,6.624477e-7,0.0000026030755,0.00009125838,0.000005064128,0.00016210813],"genre_scores_gemma":[0.9988716,0.00002758355,0.00021996674,0.000019619243,0.0000055422433,0.0000033193528,0.0005504203,0.0000042036254,0.00029761015],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999151,0.000005175371,0.000006989787,0.000027733871,0.000021719294,0.000023181577],"domain_scores_gemma":[0.99975854,0.000013280433,0.00007293241,0.000019088093,0.000023035023,0.00011317375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013657937,0.00024405494,0.0002753933,0.001066674,0.00043796396,0.0004787023,0.0002416575,0.00021967149,0.0007486113],"category_scores_gemma":[0.00016321692,0.0001506879,0.00025251321,0.0006782946,0.0002088785,0.00013439823,0.00046372585,0.00017596608,0.00030567253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013535285,0.000051650575,0.95381516,0.00001207639,0.00004295738,0.0012584829,0.00030341386,0.00009446196,0.040655192,0.000043572858,0.0001344297,0.0034533988],"study_design_scores_gemma":[0.0000021017693,0.000023126111,0.99884003,8.8275e-7,0.0000101383175,0.0004974441,0.00010820106,0.000101860234,0.00025217215,0.000009149576,0.00015337285,0.0000015061906],"about_ca_topic_score_codex":0.0070384657,"about_ca_topic_score_gemma":0.013464621,"teacher_disagreement_score":0.0070384657,"about_ca_system_score_codex":0.0002080457,"about_ca_system_score_gemma":0.00012064802,"threshold_uncertainty_score":0.013994992},"labels":[],"label_agreement":null},{"id":"W1998497506","doi":"10.1086/431542","title":"Core Overshoot: An Improved Treatment and Constraints from Seismic Data","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Overshoot (microwave communication); Limit (mathematics); Stars; Astrophysics; Physics; Core (optical fiber); Computer science; Mechanics; Mathematics; Optics; Mathematical analysis; Telecommunications","score_opus":0.04090001275034777,"score_gpt":0.2691838587330829,"score_spread":0.22828384598273516,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998497506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.765168,0.0004981966,0.22941718,0.0001771352,0.000013558126,0.000043760072,0.00060991617,0.0010627869,0.0030093463],"genre_scores_gemma":[0.936325,0.00021083851,0.06174095,0.00002785725,0.000020396763,0.000031119955,0.000657093,0.0001573892,0.00082927715],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998534,0.000022400047,0.000013943301,0.000050384635,0.000041870037,0.000018073475],"domain_scores_gemma":[0.9994093,0.0001683624,0.0001292631,0.00016626022,0.00007662663,0.000050143146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035696197,0.00054209866,0.000595692,0.00084965926,0.0003752713,0.00088119594,0.0008056951,0.0004990325,0.0007138974],"category_scores_gemma":[0.0013526195,0.000390903,0.000629126,0.0006819749,0.00037502882,0.00067488896,0.0014685764,0.0006857243,0.00017138808],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003129485,0.00007263836,0.12220602,0.00019073104,0.00010519265,0.0006341122,0.0005947453,0.7047984,0.06474182,0.010822507,0.00071177416,0.09480912],"study_design_scores_gemma":[0.000020420575,0.000067177665,0.026826227,0.000019019371,0.000021943124,0.00019856819,0.00008171931,0.9619198,0.0066961534,0.0029097544,0.001210918,0.000028280436],"about_ca_topic_score_codex":0.006889775,"about_ca_topic_score_gemma":0.0058430484,"teacher_disagreement_score":0.006889775,"about_ca_system_score_codex":0.00039536558,"about_ca_system_score_gemma":0.0004486508,"threshold_uncertainty_score":0.013699293},"labels":[],"label_agreement":null},{"id":"W1998499609","doi":"10.1086/429870","title":"A Self‐Absorption Census of Cold H<scp>i</scp>Clouds in the Canadian Galactic Plane Survey","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; University of Calgary","funders":"","keywords":"Physics; Galactic plane; Astrophysics; Interstellar medium; Stars; Astronomy; Molecular cloud; Spiral galaxy; Population; Context (archaeology); Absorption (acoustics); Radial velocity; Galaxy; Optics; Geography","score_opus":0.01513750074630796,"score_gpt":0.2350256610678775,"score_spread":0.21988816032156955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998499609","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96059895,0.0012190946,0.00029914532,0.00041424518,0.000011927212,0.00007123364,0.030145546,0.000057170848,0.0071826205],"genre_scores_gemma":[0.98042595,0.0014446503,0.000844754,0.00015363294,0.0000116905585,0.000032518154,0.014436823,0.000023054292,0.0026268791],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99937266,0.00001669568,0.000019385696,0.00009494572,0.0003080733,0.00018827798],"domain_scores_gemma":[0.9987618,0.000043408785,0.00017430261,0.000052951033,0.0005924553,0.00037510303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029659463,0.00032785427,0.0002690671,0.0037604533,0.0024523153,0.0009737149,0.0010001899,0.0002551757,0.0020659114],"category_scores_gemma":[0.00108613,0.00021586524,0.0002435575,0.007182558,0.0005721917,0.00044309555,0.00084146886,0.0002527806,0.00028639688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050549745,0.000018147632,0.9661332,0.00012108227,0.000069040216,0.0001514711,0.0014081981,0.00025904074,0.0030068473,0.00071468693,0.0096132625,0.01845443],"study_design_scores_gemma":[0.0000015549425,0.0000062880654,0.99379104,0.000010050686,0.000009547968,0.000061061364,0.00040581558,0.00017999587,0.000132209,0.000016347436,0.0053781318,0.000007919999],"about_ca_topic_score_codex":0.9916494,"about_ca_topic_score_gemma":0.9967788,"teacher_disagreement_score":0.9916494,"about_ca_system_score_codex":0.013093367,"about_ca_system_score_gemma":0.016174924,"threshold_uncertainty_score":0.09499949},"labels":[],"label_agreement":null},{"id":"W1998564561","doi":"10.1086/517604","title":"Improving the Speckle Noise Attenuation of Simultaneous Spectral Differential Imaging with a Focal Plane Holographic Diffuser","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Optics; Speckle pattern; Physics; Point spread function; Speckle noise; Holography; Diffuser (optics); Cardinal point; Adaptive optics; Noise (video); Computer science; Artificial intelligence","score_opus":0.005416596324032794,"score_gpt":0.20433010167748733,"score_spread":0.19891350535345453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998564561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86866486,0.00050219946,0.12713757,0.00014558942,0.000039863968,0.00006878155,0.000055919267,0.0006661843,0.002718943],"genre_scores_gemma":[0.82822245,0.00030137945,0.16892067,0.00010561733,0.00003082928,0.000067217166,0.00012506654,0.000082661885,0.0021441814],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9992084,0.0000832537,0.00004630956,0.00019216098,0.00040689754,0.000063043924],"domain_scores_gemma":[0.99843544,0.0005677052,0.00020921884,0.00028528072,0.00042286713,0.00007938424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009756962,0.000374544,0.00050298136,0.0005275546,0.00022479905,0.00073277496,0.0007206248,0.0004416405,0.001185421],"category_scores_gemma":[0.0018979603,0.00041391543,0.00031034616,0.00042806787,0.0004537548,0.0008387407,0.00085221825,0.0004368515,0.00034274292],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012473628,0.00007326682,0.0023777024,0.00006342329,0.000014385409,0.00007289297,0.000086086875,0.0012134303,0.9713344,0.00057834457,0.0001371062,0.023924246],"study_design_scores_gemma":[0.0000351794,0.00028259103,0.0056794984,0.0000073702486,0.000030439776,0.00030637014,0.000025341647,0.022470945,0.96931547,0.00010479118,0.001720023,0.000022070875],"about_ca_topic_score_codex":0.0010230927,"about_ca_topic_score_gemma":0.0018524517,"teacher_disagreement_score":0.001185421,"about_ca_system_score_codex":0.0006967494,"about_ca_system_score_gemma":0.0003778232,"threshold_uncertainty_score":0.0051600337},"labels":[],"label_agreement":null},{"id":"W1998588315","doi":"10.1088/0004-637x/746/1/51","title":"CONVECTIVE BURSTS AND THE COUPLING OF SATURN'S EQUATORIAL STORMS AND INTERIOR ROTATION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Saturn; Rotation (mathematics); Astronomy; Convection; Storm; Coupling (piping); Astrophysics; Astrobiology; Meteorology; Planet; Geometry","score_opus":0.005865298382841875,"score_gpt":0.22209457665140694,"score_spread":0.21622927826856506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998588315","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99340737,0.00018327907,0.0029795594,0.000085539345,0.000008791465,0.000004430604,0.000033190856,0.00004961064,0.0032482685],"genre_scores_gemma":[0.9994535,0.000061543,0.00028964714,0.000006313348,0.0000064791843,0.0000016118094,0.000021488742,0.000007838729,0.00015170775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994266,0.000014593343,0.0000042002375,0.000013821193,0.000010998974,0.000013737027],"domain_scores_gemma":[0.99964225,0.00009587617,0.00017040035,0.000030037203,0.000021418035,0.000039992567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017518176,0.0001739706,0.00012829609,0.00019629979,0.0002023589,0.00057579536,0.00014388112,0.0001498127,0.0009291862],"category_scores_gemma":[0.0013365448,0.00016216838,0.0001515022,0.00013611937,0.0003175966,0.00027332111,0.00054102216,0.00022599997,0.00008288939],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005164622,0.00013802665,0.5821699,0.00015539785,0.00025649252,0.00097163586,0.001384214,0.23408681,0.10849602,0.027341636,0.0010702846,0.04341327],"study_design_scores_gemma":[0.000045752357,0.000101074336,0.56390154,0.00001895304,0.00006177213,0.00025329253,0.00026241114,0.4175641,0.005693631,0.010297614,0.0017749683,0.000024854255],"about_ca_topic_score_codex":0.0065586795,"about_ca_topic_score_gemma":0.002630544,"teacher_disagreement_score":0.0065586795,"about_ca_system_score_codex":0.0004881693,"about_ca_system_score_gemma":0.00018233027,"threshold_uncertainty_score":0.013041019},"labels":[],"label_agreement":null},{"id":"W1998657320","doi":"10.1088/0004-637x/746/2/163","title":"THE MULTI-EPOCH NEARBY CLUSTER SURVEY: TYPE Ia SUPERNOVA RATE MEASUREMENT IN<i>z</i>∼ 0.1 CLUSTERS AND THE LATE-TIME DELAY TIME DISTRIBUTION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Supernova; Galaxy; Redshift; Cluster (spacecraft); Galaxy cluster; Star formation; Astronomy; Type (biology)","score_opus":0.017041865152540008,"score_gpt":0.2368723483601176,"score_spread":0.21983048320757761,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998657320","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98748827,0.00013872143,0.004264234,0.000040981075,0.000009940676,0.000059986327,0.0054118196,0.00023922307,0.0023469655],"genre_scores_gemma":[0.9806487,0.00009908596,0.011603772,0.00003687184,0.000017453256,0.00005167827,0.00630295,0.000050172297,0.001189382],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997546,0.000032219923,0.000013511495,0.000093233226,0.00006773081,0.000038804057],"domain_scores_gemma":[0.99899775,0.000085059495,0.00034471924,0.00015131311,0.00014334811,0.00027778026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071002526,0.00025758735,0.00017602868,0.0012480333,0.00021938556,0.00034409965,0.00047034107,0.00019780116,0.00085642486],"category_scores_gemma":[0.001045501,0.00018985837,0.00026255706,0.00086702756,0.00013849,0.0002559327,0.0005445765,0.00018524694,0.0003913894],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008127927,0.00002203223,0.9837806,0.000017511918,0.000054806093,0.00003733532,0.00009755755,0.0023348122,0.0040195873,0.00033004518,0.0012150541,0.008009327],"study_design_scores_gemma":[0.0000053260705,0.000031427193,0.9938013,0.0000033892104,0.000014841247,0.00007753767,0.000029571385,0.003472846,0.0009923298,0.0000681739,0.0014946897,0.00000849464],"about_ca_topic_score_codex":0.028816976,"about_ca_topic_score_gemma":0.065994926,"teacher_disagreement_score":0.028816976,"about_ca_system_score_codex":0.00060786185,"about_ca_system_score_gemma":0.0004500907,"threshold_uncertainty_score":0.05729848},"labels":[],"label_agreement":null},{"id":"W1998662034","doi":"10.1088/0004-637x/723/1/719","title":"DIFFUSIVE NUCLEAR BURNING OF HELIUM ON NEUTRON STARS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Neutron star; Supernova; Helium; Stars; Neutron; Thermal; Nuclear reaction; Cassiopeia A","score_opus":0.007670181054227229,"score_gpt":0.21939265785620699,"score_spread":0.21172247680197975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998662034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98786443,0.00021135966,0.00312238,0.000058867354,0.000013680826,0.000011598083,0.000101165155,0.000031657102,0.008584948],"genre_scores_gemma":[0.99784935,0.00018419727,0.0004485397,0.00001896812,0.000004740913,0.0000085581505,0.000094280316,0.0000127325775,0.0013786993],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999238,0.000011774425,0.0000045984243,0.000011224783,0.000019138186,0.000029345514],"domain_scores_gemma":[0.9998652,0.000034529174,0.000019198944,0.000015293555,0.000026204132,0.0000396274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015690917,0.0003149576,0.00033570745,0.0003769186,0.00039727235,0.0005143081,0.0004974026,0.000527052,0.0019669873],"category_scores_gemma":[0.00070316385,0.00022960344,0.00048390438,0.00025665408,0.0004702355,0.00053032173,0.0006001041,0.0002720205,0.00022662162],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029671766,0.00011948591,0.037600223,0.00011156871,0.00008264873,0.00068990665,0.00021428578,0.88254434,0.032643333,0.03742841,0.00044677334,0.007822368],"study_design_scores_gemma":[0.00006693342,0.00011542536,0.029731236,0.000029614497,0.000022665201,0.00016610476,0.00011921264,0.95524055,0.0062564192,0.007049633,0.001171251,0.000030992953],"about_ca_topic_score_codex":0.015949203,"about_ca_topic_score_gemma":0.009483281,"teacher_disagreement_score":0.015949203,"about_ca_system_score_codex":0.0013057783,"about_ca_system_score_gemma":0.00064428744,"threshold_uncertainty_score":0.03171271},"labels":[],"label_agreement":null},{"id":"W1998694524","doi":"10.1086/452628","title":"Detection of Long‐Period Variations in the Subdwarf B Star PG 0101+039 on the Basis of Photometry from the<i>MOST</i>Satellite","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; St. Mary's University; University of British Columbia; Saint Mary's University; Université de Montréal","funders":"","keywords":"Subdwarf; Physics; Photometry (optics); Astrophysics; Variable star; Brightness; Effective temperature; Spectral line; Stars; Astronomy; White dwarf","score_opus":0.011058707225671054,"score_gpt":0.21994525633005899,"score_spread":0.20888654910438792,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998694524","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939287,0.00003571157,0.00012452833,0.0000150942715,0.0000021417377,0.0000026490904,0.000084993306,0.000009314328,0.0003325979],"genre_scores_gemma":[0.9993305,0.000038730122,0.00027220213,0.0000126311215,0.000006390759,0.00000399532,0.0002715125,0.0000028657391,0.00006109937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991524,0.000009131386,0.0000058100545,0.00002908171,0.000022018952,0.000018676927],"domain_scores_gemma":[0.99947697,0.000077817356,0.00019416075,0.000051210845,0.000039526432,0.0001602851],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016224927,0.00021713784,0.00019552028,0.0005037697,0.00049097784,0.00043748162,0.0002615055,0.00038958862,0.00063145225],"category_scores_gemma":[0.000479223,0.00017567069,0.00014068333,0.00046950427,0.00035623633,0.00022542001,0.00043841757,0.00032073708,0.00024010522],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003871901,0.00007258364,0.9090964,0.000055435372,0.000050074523,0.00064976094,0.00029623855,0.00045587806,0.07755182,0.00028703196,0.00021775332,0.0108798975],"study_design_scores_gemma":[0.000014872324,0.000118021904,0.99499655,0.0000049354426,0.000017655293,0.00069388415,0.000072910545,0.00060221396,0.0028614781,0.00010491871,0.00050753646,0.0000049081664],"about_ca_topic_score_codex":0.0009414604,"about_ca_topic_score_gemma":0.0019463217,"teacher_disagreement_score":0.0009414604,"about_ca_system_score_codex":0.0002591963,"about_ca_system_score_gemma":0.00013020751,"threshold_uncertainty_score":0.0021123886},"labels":[],"label_agreement":null},{"id":"W1998731207","doi":"10.1086/421337","title":"The DEEP2 Galaxy Redshift Survey: Clustering of Galaxies in Early Data","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":180,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Galaxy; Redshift; Redshift survey; Correlation function (quantum field theory); Astronomy; Cosmic variance; Redshift-space distortions","score_opus":0.019056241932711496,"score_gpt":0.23985800952585887,"score_spread":0.22080176759314737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998731207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911271,0.00009023349,0.0010077767,0.000055480334,0.0000035370585,0.000012886057,0.006576353,0.00007505973,0.0010515108],"genre_scores_gemma":[0.9818526,0.00006111549,0.0015836837,0.000029997225,0.000011218705,0.00002102681,0.015490512,0.000022145245,0.00092772825],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99918085,0.00019238726,0.000045012424,0.00017528208,0.00024324228,0.0001631585],"domain_scores_gemma":[0.9964168,0.0003611257,0.0013104926,0.00055520615,0.00054089434,0.0008153993],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001037781,0.00039918663,0.00039329278,0.0038245453,0.00032600225,0.00070523453,0.0005970144,0.000359325,0.0012648501],"category_scores_gemma":[0.0031491166,0.00021237969,0.00033768424,0.0040202592,0.0003066866,0.00045664402,0.0012727197,0.00034357698,0.0008468606],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013045728,0.000059644877,0.98822904,0.000037167276,0.00010013101,0.00006993918,0.00017967874,0.0010101461,0.002216835,0.0004079293,0.0015297896,0.0060292385],"study_design_scores_gemma":[0.0000072446874,0.000020598121,0.99648833,0.0000033884455,0.000009647904,0.00007064165,0.000063426596,0.0012664002,0.0005414392,0.00011362184,0.0014086582,0.0000066748066],"about_ca_topic_score_codex":0.01775233,"about_ca_topic_score_gemma":0.027098773,"teacher_disagreement_score":0.01775233,"about_ca_system_score_codex":0.00089261774,"about_ca_system_score_gemma":0.0003545124,"threshold_uncertainty_score":0.03529799},"labels":[],"label_agreement":null},{"id":"W1998752294","doi":"10.1086/317244","title":"Comparison of Theory and Observations of the Chirality of Filaments within a Dispersing Activity Complex","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Differential rotation; Protein filament; Chirality (physics); Magnetic field; Field line; Polarity (international relations); Magnetic flux; Rotation (mathematics); Astrophysics; Inversion (geology); Computational physics; Geometry; Quantum mechanics; Geology; Chemistry","score_opus":0.03209802163924512,"score_gpt":0.294612711279895,"score_spread":0.2625146896406499,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998752294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9785896,0.0001067266,0.013243706,0.00016581043,0.000010640164,0.000028784938,0.0001587844,0.00014566512,0.007550272],"genre_scores_gemma":[0.99780744,0.000052744374,0.0018852863,0.0000100472,0.000003995951,0.000010528814,0.00006147147,0.000020571642,0.00014793823],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988365,0.000031340605,0.000005315349,0.00002587476,0.000029157964,0.000024494084],"domain_scores_gemma":[0.9992982,0.0003069966,0.00008913099,0.00013002178,0.0001088861,0.00006672981],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037259207,0.00030457816,0.00031450752,0.00031592147,0.00031945354,0.0006835841,0.00073990325,0.00038492642,0.00097244565],"category_scores_gemma":[0.0019231399,0.000232927,0.0003660652,0.00019968342,0.0006946854,0.0005604001,0.0002921478,0.00031734203,0.000076233],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000058972524,0.00003322498,0.012745903,0.000027824679,0.000018971743,0.000110383,0.00006213178,0.9745393,0.004596854,0.0052936515,0.00014163512,0.0023711934],"study_design_scores_gemma":[0.000018485116,0.000015934527,0.0021795728,0.00000370787,0.0000046091527,0.000012278937,0.000017368655,0.995199,0.0013092862,0.001103571,0.0001308335,0.000005261103],"about_ca_topic_score_codex":0.009219374,"about_ca_topic_score_gemma":0.0025536548,"teacher_disagreement_score":0.009219374,"about_ca_system_score_codex":0.0009877707,"about_ca_system_score_gemma":0.0004488529,"threshold_uncertainty_score":0.018331409},"labels":[],"label_agreement":null},{"id":"W1998759148","doi":"10.1086/519492","title":"Evidence that FeLoBALs May Signify the Transition between an Ultraluminous Infrared Galaxy and a Quasar","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; QSOS; Astrophysics; Luminous infrared galaxy; Astronomy; Quasar; Supermassive black hole; Galaxy; Spitzer Space Telescope; Star formation; Infrared; Redshift; Photometry (optics); Active galactic nucleus; Telescope; Stars","score_opus":0.02520879655455514,"score_gpt":0.25488846392119047,"score_spread":0.22967966736663534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998759148","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.954219,0.0008206969,0.0014965192,0.0020327773,0.00029072972,0.000016598447,0.00047362098,0.00012123417,0.040528763],"genre_scores_gemma":[0.9956607,0.00019634412,0.0005050203,0.00030041204,0.00011323261,0.000003449958,0.0001655676,0.000010379484,0.0030447969],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998374,0.000024857316,0.000011898246,0.000034145745,0.00003435056,0.00005726735],"domain_scores_gemma":[0.9967715,0.0010623875,0.0011182985,0.0003590107,0.00023695327,0.00045185754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007121361,0.00018190917,0.00011342328,0.0011726901,0.0009162788,0.0012252803,0.0004325791,0.0010017486,0.00876227],"category_scores_gemma":[0.0028820634,0.000086780055,0.0001607002,0.00062943785,0.0018361815,0.00083287945,0.0007220605,0.001026386,0.0011412482],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002121826,0.00033821506,0.80157197,0.00018222432,0.00008608226,0.011433455,0.004153082,0.00013081987,0.0788775,0.03973748,0.005963804,0.055403545],"study_design_scores_gemma":[0.0000583149,0.0003776992,0.9096521,0.0000955794,0.00006594441,0.01753661,0.0028236506,0.00031297212,0.018075427,0.0115430495,0.03941448,0.00004411569],"about_ca_topic_score_codex":0.002234508,"about_ca_topic_score_gemma":0.0028309894,"teacher_disagreement_score":0.00876227,"about_ca_system_score_codex":0.00050106895,"about_ca_system_score_gemma":0.00020205295,"threshold_uncertainty_score":0.02931273},"labels":[],"label_agreement":null},{"id":"W1998929151","doi":"10.1086/423667","title":"Nonthermal Radiation Processes in X-Ray Jets","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Equipartition theorem; Synchrotron radiation; Synchrotron; Knot (papermaking); Doppler effect; Magnetic field; Jet (fluid)","score_opus":0.006357978715607691,"score_gpt":0.21658570260857402,"score_spread":0.21022772389296632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998929151","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6156983,0.0023115163,0.36277035,0.0003833572,0.00006452178,0.000049752744,0.00010406721,0.00031784063,0.01830028],"genre_scores_gemma":[0.9889626,0.000565473,0.0070112697,0.000038655297,0.000059617523,0.00003051253,0.00006233954,0.000052866224,0.0032166059],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9995864,0.00017449542,0.00002074489,0.000045136763,0.00010766911,0.00006549728],"domain_scores_gemma":[0.9983658,0.0010303642,0.00027688406,0.00014691787,0.00010879613,0.000071288894],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078602455,0.0006257238,0.00034761464,0.0006949049,0.00055202463,0.0018143135,0.0009055755,0.00043148015,0.0015573329],"category_scores_gemma":[0.0052566165,0.00039960508,0.00059354265,0.0005056358,0.0010526838,0.0015997865,0.00086055987,0.0006102889,0.00031507562],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001698374,0.00008780129,0.021066893,0.00013395605,0.000058871265,0.0010215336,0.00043070503,0.5283109,0.015556671,0.41230628,0.0007259385,0.02013069],"study_design_scores_gemma":[0.000039628736,0.00006410663,0.0060562333,0.000018640178,0.000022622711,0.00054471724,0.0001085065,0.8772825,0.0032109753,0.11159261,0.0010305429,0.000028897384],"about_ca_topic_score_codex":0.0012575304,"about_ca_topic_score_gemma":0.0010757564,"teacher_disagreement_score":0.0018143135,"about_ca_system_score_codex":0.0009230544,"about_ca_system_score_gemma":0.00030728398,"threshold_uncertainty_score":0.0066972375},"labels":[],"label_agreement":null},{"id":"W1998948355","doi":"10.1086/324193","title":"Tidal Evolution of the Planetary System around HD 83443","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Planet; Exoplanet; Tidal acceleration; Angular momentum; Astronomy; Eccentricity (behavior); Orbital period; Orbital eccentricity; Astrophysics; RADIUS; Planetary system; Orbital decay; Tidal heating; Perturbation (astronomy); Circular orbit; Stars; Classical mechanics; Satellite","score_opus":0.010353130207320597,"score_gpt":0.18740483181601353,"score_spread":0.17705170160869294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1998948355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978771,0.000038118425,0.00007841417,0.000025874875,0.0000032653568,0.0000026345494,0.0002107704,0.000020111744,0.0017438154],"genre_scores_gemma":[0.9989563,0.000019675565,0.000116643314,0.00001106948,0.0000022841182,0.0000020129494,0.00042920603,0.000005604317,0.00045722266],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999503,0.000005093749,0.0000023655875,0.000009501596,0.000016046493,0.00001658937],"domain_scores_gemma":[0.99988735,0.000009892088,0.000027241653,0.000010755224,0.00003174002,0.000032972843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000095235024,0.00012387015,0.00018063515,0.0003727107,0.0006323484,0.0003500713,0.0001448074,0.00022114824,0.0012250365],"category_scores_gemma":[0.0003357124,0.00008991285,0.00014859259,0.00063433795,0.00021513682,0.00013302595,0.00043605707,0.00023818966,0.00042766938],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042596975,0.00017742523,0.83018404,0.000062640596,0.00013981039,0.0011982869,0.0013480324,0.0060236906,0.119129814,0.0019515408,0.0041964003,0.035162326],"study_design_scores_gemma":[0.000005027609,0.00003283388,0.99524236,0.0000025778675,0.000008772497,0.00015155903,0.00008044266,0.0021569526,0.00096527836,0.00008721723,0.0012601038,0.000007004029],"about_ca_topic_score_codex":0.018947428,"about_ca_topic_score_gemma":0.014899945,"teacher_disagreement_score":0.018947428,"about_ca_system_score_codex":0.0006528511,"about_ca_system_score_gemma":0.00027474345,"threshold_uncertainty_score":0.03767425},"labels":[],"label_agreement":null},{"id":"W1999144042","doi":"10.1086/318990","title":"Simulations of Accretion Flows Crossing the Last Stable Orbit","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Magnetohydrodynamic drive; Angular momentum; Magnetohydrodynamics; Accretion (finance); Circular orbit; Magnetic field; Orbit (dynamics); Accretion disc; Point (geometry)","score_opus":0.018684911991396335,"score_gpt":0.2560903907499945,"score_spread":0.2374054787585982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999144042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99469876,0.00006692755,0.0019339015,0.00017276675,0.000016293356,0.000030670253,0.0002495778,0.00008732036,0.0027438577],"genre_scores_gemma":[0.9968629,0.00004448978,0.0024180592,0.000037354876,0.0000072337384,0.000033736924,0.00025373715,0.000021778622,0.0003207278],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998511,0.00003147263,0.000009595351,0.000023330995,0.000030021569,0.00005437199],"domain_scores_gemma":[0.99887913,0.00055919396,0.00012855911,0.0000569175,0.00011932485,0.00025685513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000363373,0.00047986567,0.00063892134,0.0005568946,0.000837098,0.0008106793,0.0009311514,0.0011585966,0.0011983031],"category_scores_gemma":[0.0022202788,0.0003740036,0.0005517719,0.00067845616,0.00093370955,0.00054046675,0.0007353563,0.0010217885,0.0000948455],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028999246,0.00017606284,0.008838975,0.000039577946,0.00006559142,0.0002825835,0.00018565747,0.9826889,0.0028617245,0.0024317536,0.00039238445,0.0017467438],"study_design_scores_gemma":[0.00007559605,0.000065838336,0.0019508883,0.000006014768,0.000011614619,0.00002117784,0.000057535068,0.9963038,0.0007172257,0.0005760054,0.00020370037,0.000010589885],"about_ca_topic_score_codex":0.015079425,"about_ca_topic_score_gemma":0.00831156,"teacher_disagreement_score":0.015079425,"about_ca_system_score_codex":0.0009882909,"about_ca_system_score_gemma":0.0007296045,"threshold_uncertainty_score":0.029983342},"labels":[],"label_agreement":null},{"id":"W1999249763","doi":"10.1088/0004-637x/704/2/1616","title":"WATER, METHANE, AND CARBON DIOXIDE PRESENT IN THE DAYSIDE SPECTRUM OF THE EXOPLANET HD 209458b","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":291,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Exoplanet; Physics; Astrophysics; Methane; Carbon dioxide; Infrared; Spectral resolution; Spectral line; Planet; Astronomy; Chemistry","score_opus":0.00938572519910894,"score_gpt":0.21611945619386758,"score_spread":0.20673373099475864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999249763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937785,0.000024335695,0.00006406113,0.000010911855,0.0000013531601,0.0000013204057,0.0001631034,0.0000066805833,0.00035040063],"genre_scores_gemma":[0.99910754,0.000022546312,0.00023098962,0.000012817828,0.0000043785158,0.0000022357663,0.0004985145,0.0000047325348,0.00011629041],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999114,0.000008134801,0.0000052929663,0.000034262543,0.000021485614,0.000019520345],"domain_scores_gemma":[0.9998599,0.000015215965,0.000038872226,0.000017494005,0.000027048074,0.000041462223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015490125,0.00023519817,0.00021324896,0.0006467205,0.00037426432,0.00040230533,0.00021156539,0.00024020366,0.0005308638],"category_scores_gemma":[0.00028137147,0.0002040743,0.00014096533,0.00034380914,0.0002667654,0.00034086907,0.00042141098,0.00019612318,0.000116722396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007020601,0.0001873733,0.7437483,0.000049924416,0.0001695292,0.0006860566,0.0006324585,0.00087564485,0.2428712,0.0004706408,0.00041890188,0.009187967],"study_design_scores_gemma":[0.000018346238,0.000045992605,0.99049735,0.0000048268116,0.00002003134,0.0001988595,0.00009432894,0.000759216,0.007669993,0.00007911691,0.00060450804,0.000007409271],"about_ca_topic_score_codex":0.003197206,"about_ca_topic_score_gemma":0.005752139,"teacher_disagreement_score":0.003197206,"about_ca_system_score_codex":0.0003151246,"about_ca_system_score_gemma":0.00009542538,"threshold_uncertainty_score":0.006357193},"labels":[],"label_agreement":null},{"id":"W1999350262","doi":"10.1086/429255","title":"The Discovery of More than 2000 White Dwarfs in the Globular Cluster ω Centauri","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; White dwarf; Physics; Hubble space telescope; Astrophysics; Astronomy; Horizontal branch; Cluster (spacecraft); Stars; Computer science","score_opus":0.00674076367263106,"score_gpt":0.2225285867514248,"score_spread":0.21578782307879374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999350262","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99897826,0.00031438185,0.00013568463,0.000030446226,0.000007318566,0.000001299742,0.00009511865,0.000010968326,0.00042658582],"genre_scores_gemma":[0.9988709,0.00015876404,0.00021100506,0.000038724236,0.000021020516,0.0000017342869,0.00036457254,0.0000026950147,0.00033037874],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983656,0.000007961418,0.000008380865,0.00006390512,0.000040789506,0.000042479467],"domain_scores_gemma":[0.9994311,0.00008619577,0.00018877767,0.00006155671,0.000042150845,0.00019027153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002912609,0.00020248185,0.00013553163,0.0015547444,0.0004299206,0.0006652197,0.00022305262,0.00031576847,0.00055560516],"category_scores_gemma":[0.00067899015,0.00014511746,0.000097485616,0.0008031015,0.00050034566,0.00045847346,0.00076087145,0.00019405488,0.00019602072],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018325604,0.000047689482,0.92451763,0.00007239955,0.00007442328,0.0009763864,0.001075661,0.00018542768,0.037118252,0.0006563972,0.00095068495,0.034141812],"study_design_scores_gemma":[0.0000033049405,0.00003887828,0.9961074,0.000007775715,0.000018996703,0.0006016962,0.00013680039,0.000105819585,0.0011772419,0.00014933031,0.0016469639,0.0000056866866],"about_ca_topic_score_codex":0.0016265467,"about_ca_topic_score_gemma":0.003094438,"teacher_disagreement_score":0.0016265467,"about_ca_system_score_codex":0.0002792421,"about_ca_system_score_gemma":0.00011483916,"threshold_uncertainty_score":0.003234148},"labels":[],"label_agreement":null},{"id":"W1999356207","doi":"10.1086/375264","title":"Karhunen‐Loeve Estimation of the Power Spectrum Parameters from the Angular Distribution of Galaxies in Early Sloan Digital Sky Survey Data","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Galaxy; Physics; Sky; Spectral density; Astrophysics; Scaling; Data set; Limiting magnitude; Magnitude (astronomy); Statistical physics; Statistics; Mathematics; Geometry","score_opus":0.011558103778472545,"score_gpt":0.21326541082829648,"score_spread":0.20170730704982393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999356207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93012166,0.00021942538,0.06741204,0.00014042151,0.0000043445393,0.0000154662,0.00051534653,0.00029700145,0.0012742999],"genre_scores_gemma":[0.9783705,0.00008865854,0.020665089,0.000015645133,0.000008125557,0.000020426029,0.000645605,0.000029458088,0.00015647079],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99937797,0.0002765746,0.000041919833,0.00009769267,0.00013611992,0.00006961428],"domain_scores_gemma":[0.99691063,0.0016245933,0.00043751762,0.00063110475,0.0002757145,0.00012039643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020249265,0.00041281778,0.00023662331,0.0013408426,0.00031430039,0.00094012165,0.00045819758,0.00027188723,0.00056539156],"category_scores_gemma":[0.011275804,0.0002502192,0.00029955123,0.0008288677,0.0005050915,0.00067867606,0.0007346089,0.00034162545,0.00019372045],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003391457,0.000085856984,0.5066153,0.00018788246,0.00034066144,0.0002816348,0.00084593357,0.24589863,0.033324327,0.020674625,0.0018734881,0.1895326],"study_design_scores_gemma":[0.00003250865,0.00003477924,0.5018616,0.000037161328,0.000043114145,0.00022653732,0.0001531922,0.47266155,0.011766415,0.011176607,0.0018983057,0.000108264154],"about_ca_topic_score_codex":0.01086114,"about_ca_topic_score_gemma":0.011622938,"teacher_disagreement_score":0.01086114,"about_ca_system_score_codex":0.0007063467,"about_ca_system_score_gemma":0.0005499125,"threshold_uncertainty_score":0.021595836},"labels":[],"label_agreement":null},{"id":"W1999358632","doi":"10.1088/0004-637x/737/1/8","title":"THE GENESIS OF THE MILKY WAY'S THICK DISK VIA STELLAR MIGRATION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":253,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Thick disk; Milky Way; Physics; Astrophysics; Stars; Thin disk; Metallicity; Galaxy; Astronomy; Halo","score_opus":0.013958320522736661,"score_gpt":0.20583373376987887,"score_spread":0.19187541324714222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999358632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962379,0.00011113389,0.0011992278,0.00013825878,0.000009695706,0.000009938932,0.00006714518,0.000029197803,0.002197576],"genre_scores_gemma":[0.9988489,0.000087581975,0.0005297669,0.000023332987,0.000004515612,0.0000055175733,0.00003914929,0.000009240787,0.0004519451],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993515,0.000019428671,0.0000033093925,0.000013989263,0.0000091794145,0.000018882507],"domain_scores_gemma":[0.9997639,0.000044406614,0.000058082587,0.000028611657,0.000023869714,0.000081237355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024992807,0.00028498244,0.0003221885,0.00031813723,0.0004782086,0.0011709287,0.00055907137,0.00064955524,0.0011943841],"category_scores_gemma":[0.0013235348,0.0002309423,0.000439311,0.00021287477,0.00061596424,0.000992304,0.0008248582,0.00036933302,0.0001559324],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089841895,0.00024689749,0.37831375,0.00028655338,0.00035537564,0.0020464405,0.0016765302,0.53572947,0.019880569,0.043774452,0.0016813513,0.015110228],"study_design_scores_gemma":[0.00038455034,0.00045396917,0.18494548,0.000081748,0.0001327273,0.0005770456,0.0010012226,0.7902296,0.0025469845,0.014788825,0.0047738566,0.00008392389],"about_ca_topic_score_codex":0.012927164,"about_ca_topic_score_gemma":0.0075587146,"teacher_disagreement_score":0.012927164,"about_ca_system_score_codex":0.00076659,"about_ca_system_score_gemma":0.00051111245,"threshold_uncertainty_score":0.025703847},"labels":[],"label_agreement":null},{"id":"W1999383621","doi":"10.1086/512599","title":"A Systematic Search for High Surface Brightness Giant Arcs in a Sloan Digital Sky Survey Cluster Sample","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Sky; Surface brightness; Arc (geometry); Brightness; Cluster (spacecraft); Astrophysics; Sample (material); Galaxy; Selection (genetic algorithm); Physics; Computer science; Computer graphics (images); Optics; Artificial intelligence; Mathematics; Geometry","score_opus":0.0128179462690164,"score_gpt":0.2397562970568251,"score_spread":0.22693835078780872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999383621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99828833,0.000087159475,0.00027001277,0.000014237772,0.0000012203527,0.000020588092,0.0008743175,0.000027347434,0.00041676898],"genre_scores_gemma":[0.99544877,0.00007327521,0.0011598163,0.00001924828,0.000004346684,0.00002286479,0.002891457,0.000013541165,0.00036673193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992656,0.00010646827,0.000065269465,0.00022472047,0.0002024915,0.00013535334],"domain_scores_gemma":[0.99723524,0.00046546702,0.00090999756,0.00047716874,0.00043900777,0.0004731534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010019634,0.0002629466,0.00025477822,0.003779614,0.0008696533,0.0006461839,0.0004146927,0.0001924775,0.0007753467],"category_scores_gemma":[0.0020565141,0.00023084343,0.00021370164,0.0032355357,0.0005380248,0.00025128308,0.0010926526,0.00015480322,0.00024339503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015749787,0.000032178334,0.98181605,0.000061517734,0.00007568024,0.00017638874,0.00047235892,0.00041458497,0.006630102,0.00020859865,0.00084015244,0.009114792],"study_design_scores_gemma":[0.00000813053,0.00002734091,0.9972928,0.000004761298,0.000028363997,0.0001317088,0.00016428233,0.0005527661,0.00091713783,0.00005787408,0.00080808403,0.0000067322158],"about_ca_topic_score_codex":0.0196835,"about_ca_topic_score_gemma":0.05445774,"teacher_disagreement_score":0.0196835,"about_ca_system_score_codex":0.0006643865,"about_ca_system_score_gemma":0.0010903686,"threshold_uncertainty_score":0.0391379},"labels":[],"label_agreement":null},{"id":"W1999519547","doi":"10.1086/529068","title":"Evidence for Merger Remnants in Early‐Type Host Galaxies of Low‐Redshift QSOs1","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":158,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Galaxy; Redshift; Luminosity; Host (biology); Astronomy; Galaxy formation and evolution; Ecology; Biology","score_opus":0.027571368492394735,"score_gpt":0.2546741221904561,"score_spread":0.22710275369806138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999519547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99940264,0.00016072454,0.00017154869,0.000010724635,0.0000010371685,0.000003584979,0.000036497353,0.000012520708,0.0002006891],"genre_scores_gemma":[0.9996811,0.000028423572,0.00014396942,0.0000064159667,0.0000040662712,0.0000015410072,0.000089217625,0.0000014720165,0.0000437391],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997571,0.000043560627,0.000020172572,0.000044640787,0.00004943778,0.00008506598],"domain_scores_gemma":[0.99821895,0.000345052,0.0007445507,0.0001345916,0.00016909913,0.00038774154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069086696,0.0003064595,0.00032683564,0.0012968348,0.000656681,0.0010135054,0.000513006,0.00046404338,0.0011866253],"category_scores_gemma":[0.0012346596,0.00034264688,0.0002713271,0.00057492673,0.00087640254,0.0005030746,0.00078012137,0.00027207262,0.0002570775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026840164,0.00007102318,0.95553833,0.00003490781,0.0000418702,0.00064318854,0.00070139254,0.00024018537,0.038756054,0.00030819597,0.00007901777,0.003317447],"study_design_scores_gemma":[0.000009684309,0.00015727858,0.99679726,0.0000042338365,0.000020831429,0.00053145195,0.00021564332,0.00043978673,0.0015425326,0.00007495429,0.00020036359,0.0000060527705],"about_ca_topic_score_codex":0.0035452498,"about_ca_topic_score_gemma":0.0037165126,"teacher_disagreement_score":0.0035452498,"about_ca_system_score_codex":0.00032408777,"about_ca_system_score_gemma":0.0001397176,"threshold_uncertainty_score":0.0070492625},"labels":[],"label_agreement":null},{"id":"W1999533780","doi":"10.1088/0004-637x/767/1/27","title":"DETECTION OF MOLECULAR ABSORPTION IN THE DAYSIDE OF EXOPLANET 51 PEGASI b?","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Exoplanet; Planet; Physics; Atmosphere (unit); Spectral resolution; Astrophysics; Transit (satellite); Spectral line; Astronomy; Meteorology","score_opus":0.007286552232808477,"score_gpt":0.2039492897537587,"score_spread":0.19666273752095023,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999533780","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99781835,0.000064755564,0.00016122154,0.000036241396,0.0000037906636,0.000005804144,0.0001828919,0.000044150656,0.0016827964],"genre_scores_gemma":[0.9985936,0.000039614544,0.00039374715,0.000032456333,0.000006647598,0.000004474971,0.0005252556,0.000008682199,0.00039548392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999242,0.000005085472,0.0000030696633,0.000034161345,0.000016318734,0.000017185464],"domain_scores_gemma":[0.9999006,0.0000070825795,0.00003879241,0.000014417616,0.0000078037765,0.000031444364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008870177,0.00020071075,0.0001629378,0.00036102344,0.00028090295,0.00033596117,0.00029202277,0.000423603,0.0009167429],"category_scores_gemma":[0.0001941602,0.00016050771,0.00017800955,0.00016735439,0.00013492868,0.00025394952,0.00033667378,0.00031101942,0.00030598365],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007985991,0.00019101634,0.569099,0.00007753205,0.00012755339,0.0007537412,0.0007565069,0.00049885834,0.40164664,0.00039613567,0.001378252,0.024276113],"study_design_scores_gemma":[0.0000084124895,0.00012837029,0.99195474,0.0000041199405,0.00001556042,0.00022691257,0.00006469846,0.0006172125,0.0054416424,0.00003857887,0.0014952378,0.0000044681115],"about_ca_topic_score_codex":0.0027934043,"about_ca_topic_score_gemma":0.005768781,"teacher_disagreement_score":0.0027934043,"about_ca_system_score_codex":0.00028961527,"about_ca_system_score_gemma":0.00006828859,"threshold_uncertainty_score":0.0055543184},"labels":[],"label_agreement":null},{"id":"W1999563842","doi":"10.1086/590542","title":"The Luminosity Dependence of the Galaxy Merger Rate","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University","funders":"","keywords":"Galaxy; Luminosity; Sky; Absolute magnitude; Luminosity function; Magnitude (astronomy); Galaxy merger; Range (aeronautics)","score_opus":0.009078267749342953,"score_gpt":0.2041027074442663,"score_spread":0.19502443969492336,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999563842","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941299,0.00015891177,0.0026595108,0.00010114108,0.0000061037886,0.00001069466,0.0005194278,0.0001681944,0.002246111],"genre_scores_gemma":[0.99811614,0.00003875698,0.0010297906,0.000019325975,0.0000027872898,0.0000053185627,0.00050405477,0.000029270459,0.00025461445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996902,0.00009085525,0.000016849413,0.000099678546,0.00004991507,0.00005262377],"domain_scores_gemma":[0.99680847,0.0014860256,0.0006336978,0.0004124203,0.00040151417,0.0002578307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010643805,0.0002447074,0.00036603727,0.0007778836,0.00028425848,0.0006507774,0.0005253029,0.00047311207,0.0016045284],"category_scores_gemma":[0.008058026,0.00026002747,0.000441643,0.000654599,0.00036211716,0.0008323368,0.00062002864,0.000563869,0.00036982473],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029425637,0.00011006583,0.57907116,0.00010180377,0.00022042157,0.00029398064,0.00034955723,0.38126212,0.018542279,0.005594135,0.00150162,0.0126585495],"study_design_scores_gemma":[0.000043778113,0.00017471344,0.22195272,0.00001850529,0.000050656043,0.00041274508,0.00010740384,0.7646203,0.009450772,0.0017309124,0.0013681294,0.000069397385],"about_ca_topic_score_codex":0.009647802,"about_ca_topic_score_gemma":0.0078018536,"teacher_disagreement_score":0.009647802,"about_ca_system_score_codex":0.00069181935,"about_ca_system_score_gemma":0.00026789933,"threshold_uncertainty_score":0.019183338},"labels":[],"label_agreement":null},{"id":"W1999645744","doi":"10.1088/0004-637x/802/1/37","title":"DISCOVERY AND CHARACTERIZATION OF WIDE BINARY SYSTEMS WITH A VERY LOW MASS COMPONENT","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Proper motion; Binary number; Stellar classification; Low Mass; Component (thermodynamics); Binary system; Characterization (materials science)","score_opus":0.009925304934519793,"score_gpt":0.19586946337514083,"score_spread":0.18594415844062104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999645744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988856,0.0002535241,0.0002998656,0.000010938531,0.0000019564482,0.0000046127548,0.000044985347,0.0000073119154,0.00049134676],"genre_scores_gemma":[0.998777,0.00006811281,0.0006782875,0.00001701682,0.000006602868,0.0000034601187,0.0002622695,0.0000020693828,0.00018522785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997714,0.00002017667,0.000025350213,0.000078663485,0.00006375019,0.000040544888],"domain_scores_gemma":[0.9994272,0.0001026948,0.00022796399,0.00006320836,0.000047322683,0.00013171392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030668426,0.00015382413,0.0002635432,0.001326355,0.00069060334,0.00087229186,0.00034410247,0.0002570574,0.0009014656],"category_scores_gemma":[0.0009445524,0.00011871391,0.00011458003,0.000651997,0.00037478292,0.0003173499,0.0006784788,0.0002466546,0.0004660655],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016701034,0.00010223556,0.87610507,0.000050835013,0.00003273106,0.0009325114,0.00042328754,0.000088452114,0.09676779,0.0002455525,0.00017884423,0.024905687],"study_design_scores_gemma":[0.000011116901,0.00018077214,0.98270345,0.0000075379994,0.000031658416,0.003059282,0.00014568317,0.00039696263,0.011152948,0.00015352132,0.0021472238,0.00000984224],"about_ca_topic_score_codex":0.00075161,"about_ca_topic_score_gemma":0.0013947996,"teacher_disagreement_score":0.001326355,"about_ca_system_score_codex":0.00022800331,"about_ca_system_score_gemma":0.00015776326,"threshold_uncertainty_score":0.003015697},"labels":[],"label_agreement":null},{"id":"W1999698634","doi":"10.1088/0004-637x/757/1/43","title":"NEAR-INFRARED SURVEY OF THE GOODS-NORTH FIELD: SEARCH FOR LUMINOUS GALAXY CANDIDATES AT<i>z</i>≳ 6.5<sup>,</sup>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Galaxy; Redshift; Astrophysics; Stars; Photometric redshift; Astronomy; Stellar mass; Star formation; Subaru Telescope; Solar mass; Hubble Ultra-Deep Field; Hubble Deep Field; Spectral line","score_opus":0.013636370249304672,"score_gpt":0.23380066426840607,"score_spread":0.2201642940191014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999698634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9746414,0.00040395017,0.0015403455,0.00015076403,0.000021130907,0.00006290674,0.012223691,0.00025363534,0.0107021555],"genre_scores_gemma":[0.94699675,0.00030214258,0.006617255,0.00021626047,0.00006725016,0.000073901145,0.03870627,0.000049493803,0.0069706356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983513,0.000013011765,0.000009111969,0.00004193969,0.000053428623,0.000047479225],"domain_scores_gemma":[0.999532,0.000028103723,0.00014170556,0.000048298672,0.00009824845,0.00015164891],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027818527,0.00017529304,0.00014327094,0.0011335107,0.00023156207,0.00029105716,0.00034777704,0.00016880543,0.0030188204],"category_scores_gemma":[0.00025227858,0.00009795656,0.00015118992,0.00074134476,0.00014663389,0.00016337464,0.0004135656,0.00014033592,0.0013870139],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015795753,0.00007469224,0.94862026,0.00010476281,0.000036344787,0.00025506222,0.00031186955,0.0002345371,0.016710991,0.00034529468,0.008854212,0.02429405],"study_design_scores_gemma":[0.0000044111384,0.000025476944,0.9914691,0.0000065958725,0.000014111241,0.00010639516,0.00014260331,0.0002240085,0.0010975089,0.000044606313,0.006862251,0.0000028367278],"about_ca_topic_score_codex":0.0071174917,"about_ca_topic_score_gemma":0.022816665,"teacher_disagreement_score":0.0071174917,"about_ca_system_score_codex":0.00028829678,"about_ca_system_score_gemma":0.00026084765,"threshold_uncertainty_score":0.01415211},"labels":[],"label_agreement":null},{"id":"W1999799480","doi":"10.1086/342366","title":"Discovery of Cyclotron Resonance Features in the Soft Gamma Repeater SGR 1806−20","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Physics; Magnetar; Cyclotron resonance; Cyclotron; Neutron star; Pulsar; Astrophysics; Electron cyclotron resonance; Accretion (finance); Magnetic field; Electron; Atomic physics; Nuclear physics","score_opus":0.011518670653559885,"score_gpt":0.2822401461853951,"score_spread":0.27072147553183523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999799480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992812,0.000080020734,0.00007429426,0.00001277758,0.000003091225,0.0000031421034,0.000055769633,0.000014992411,0.00047474878],"genre_scores_gemma":[0.9990169,0.000053283788,0.00029552277,0.000036424404,0.000013641526,0.0000035871853,0.0002829798,0.00000965587,0.0002879571],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992657,0.0000051298002,0.0000045478555,0.000028492084,0.000019043131,0.000016195238],"domain_scores_gemma":[0.9997224,0.000028961584,0.00013434207,0.0000247637,0.000024504108,0.00006493886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014286481,0.0002568051,0.00018432931,0.0005613805,0.00026584725,0.00045545478,0.00038419006,0.00044983657,0.0009311097],"category_scores_gemma":[0.00030756328,0.00014620749,0.0001450036,0.00025762714,0.00030014155,0.00013295177,0.000423832,0.0002394685,0.00043793998],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008013341,0.0001367046,0.45034146,0.00009514885,0.00006502692,0.0058065588,0.0008767174,0.00014634212,0.52770925,0.0002615926,0.00042752226,0.013332224],"study_design_scores_gemma":[0.00003216828,0.0006554114,0.96622324,0.000010632422,0.00004886541,0.008038098,0.00030270946,0.00041945645,0.020786786,0.00015828242,0.0033084543,0.00001588459],"about_ca_topic_score_codex":0.00042409918,"about_ca_topic_score_gemma":0.00076187996,"teacher_disagreement_score":0.0009311097,"about_ca_system_score_codex":0.00013766895,"about_ca_system_score_gemma":0.00006041496,"threshold_uncertainty_score":0.0031148791},"labels":[],"label_agreement":null},{"id":"W1999826014","doi":"10.1088/0004-637x/756/2/109","title":"ENERGY CONSERVATION AND GRAVITY WAVES IN SOUND-PROOF TREATMENTS OF STELLAR INTERIORS. PART I. ANELASTIC APPROXIMATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Tachocline; Physics; Adiabatic process; Dynamo; Mach number; Radiative transfer; Classical mechanics; Mechanics; Stratification (seeds); Solar dynamo; Magnetohydrodynamics; Convection; Astrophysics; Dynamo theory; Convection zone; Magnetic field; Thermodynamics","score_opus":0.011604598713286512,"score_gpt":0.22986605043040617,"score_spread":0.21826145171711966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999826014","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.042106774,0.00418724,0.8707255,0.0030974848,0.0008875403,0.00012563172,0.00027247678,0.00025397338,0.078343354],"genre_scores_gemma":[0.58450085,0.0051754476,0.3449141,0.0020693438,0.0017244607,0.00045575763,0.00039033982,0.00076198275,0.06000765],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996542,0.00015206488,0.000020674204,0.000026934074,0.00012004797,0.000026161426],"domain_scores_gemma":[0.9993666,0.00026799762,0.00010048415,0.00012794872,0.00009335698,0.000043632528],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011043277,0.0007722699,0.00043812115,0.00070474774,0.000702057,0.0011387119,0.0011157879,0.0011121813,0.0030010596],"category_scores_gemma":[0.0029821002,0.00031495548,0.0009853683,0.000487763,0.0023363305,0.0026107535,0.0019622787,0.002095441,0.00065411686],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000011006172,0.000021075244,0.0003775367,0.00005982015,0.000011096674,0.00008679625,0.0002522149,0.048124142,0.0015060514,0.94037116,0.0020888366,0.0070902957],"study_design_scores_gemma":[0.000020152727,0.000028347144,0.00047453045,0.000060974486,0.000008975931,0.000055131,0.00009326672,0.45719317,0.00061764964,0.52512646,0.016303556,0.000017682387],"about_ca_topic_score_codex":0.003716991,"about_ca_topic_score_gemma":0.0026826616,"teacher_disagreement_score":0.003716991,"about_ca_system_score_codex":0.00097502524,"about_ca_system_score_gemma":0.0006625509,"threshold_uncertainty_score":0.010039568},"labels":[],"label_agreement":null},{"id":"W1999886869","doi":"10.1088/0004-637x/757/1/27","title":"SECULAR EVOLUTION OF COMPACT BINARIES NEAR MASSIVE BLACK HOLES: GRAVITATIONAL WAVE SOURCES AND OTHER EXOTICA","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":427,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gravitational wave; Neutron star; LIGO; Stars; Compact star; Binary black hole; Binary star; Population; Perturbation (astronomy); Orbit (dynamics)","score_opus":0.01729960841552548,"score_gpt":0.2903881570950093,"score_spread":0.27308854867948384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999886869","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99696416,0.00079741486,0.00061009714,0.000048180886,0.0000066819052,0.0000026177322,0.00023964711,0.000018108372,0.0013130952],"genre_scores_gemma":[0.9986027,0.00019342155,0.00025210527,0.000015190543,0.000008572686,0.0000017961135,0.0003432369,0.000010893725,0.00057217357],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993896,0.000006361925,0.0000027161484,0.00002103278,0.000011051937,0.000019785508],"domain_scores_gemma":[0.9996946,0.000028766468,0.00013796125,0.000018141001,0.00003552906,0.000085015155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018330802,0.00018030475,0.00023912305,0.00077626744,0.000358369,0.0007780022,0.00021376746,0.00023305917,0.0018687504],"category_scores_gemma":[0.0004580408,0.00010411113,0.00013138787,0.00060729374,0.00022950232,0.00050960877,0.0006320161,0.00022181554,0.00046972322],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035826044,0.000061683626,0.93264496,0.00005655557,0.00007824784,0.0007680768,0.00041116562,0.004146082,0.02782432,0.0033906722,0.0006786226,0.029581338],"study_design_scores_gemma":[0.000008274208,0.000061540406,0.98105913,0.000017049611,0.00002785736,0.0006751944,0.00021580941,0.011884153,0.0026388369,0.0015223912,0.0018737575,0.000016057664],"about_ca_topic_score_codex":0.0022426099,"about_ca_topic_score_gemma":0.0021787777,"teacher_disagreement_score":0.0022426099,"about_ca_system_score_codex":0.0003200916,"about_ca_system_score_gemma":0.00012878847,"threshold_uncertainty_score":0.006251633},"labels":[],"label_agreement":null},{"id":"W1999951055","doi":"10.1088/0004-637x/726/1/37","title":"THE 2006 OUTBURST OF THE MAGNETAR CXOU J164710.2 – 455216","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Glitch; Magnetar; Neutron star; Flux (metallurgy); Light curve; Exponential decay; Exponential function; Stars","score_opus":0.006120403505924727,"score_gpt":0.2080022263839668,"score_spread":0.20188182287804207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W1999951055","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99770796,0.00018010125,0.00013832236,0.0000550454,0.000040450097,0.000017346623,0.00080151553,0.000025981924,0.0010332849],"genre_scores_gemma":[0.9918624,0.00040844438,0.00094295543,0.00014916222,0.00011908591,0.000029843426,0.0053788503,0.000022446922,0.0010868944],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999846,0.000014488515,0.00001375182,0.000040884373,0.000043393582,0.000041485615],"domain_scores_gemma":[0.99891067,0.000060888826,0.00052698783,0.000095405005,0.00013053557,0.00027554616],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036509457,0.00044243142,0.0005675691,0.0008146558,0.0006286102,0.0005531594,0.0003278114,0.0004663473,0.0006260149],"category_scores_gemma":[0.0007464941,0.0001675,0.000199148,0.0004611041,0.00029259518,0.0003622283,0.0007938471,0.00053140125,0.0002961383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015697313,0.00044738041,0.8633849,0.0002409853,0.0001883602,0.004231322,0.0013751759,0.001211344,0.08455124,0.00071626034,0.005231158,0.036852192],"study_design_scores_gemma":[0.000023290546,0.0002828184,0.99141425,0.000021868678,0.00003226924,0.0007786022,0.000121731755,0.00055691943,0.0020386796,0.00007521486,0.0046346313,0.000019675927],"about_ca_topic_score_codex":0.0058586635,"about_ca_topic_score_gemma":0.018731888,"teacher_disagreement_score":0.0058586635,"about_ca_system_score_codex":0.00038939388,"about_ca_system_score_gemma":0.00027516394,"threshold_uncertainty_score":0.011649132},"labels":[],"label_agreement":null},{"id":"W2000031890","doi":"10.1088/0004-637x/784/1/37","title":"16 yr OF<i>RXTE</i>MONITORING OF FIVE ANOMALOUS X-RAY PULSARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":160,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Glitch; Pulsar; Physics; Astrophysics; Radiative transfer; Flux (metallurgy); Astronomy; Detector","score_opus":0.009572254138373872,"score_gpt":0.29466074795445735,"score_spread":0.2850884938160835,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000031890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98492754,0.00048675507,0.001260743,0.00010317934,0.00003576098,0.00006691246,0.0076358803,0.00017814519,0.0053049964],"genre_scores_gemma":[0.9718992,0.0003255046,0.0021855156,0.00014423777,0.00008865265,0.00006337913,0.021827038,0.00004009764,0.003426273],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998105,0.000014549588,0.000026391417,0.000063557265,0.000042720574,0.000042414806],"domain_scores_gemma":[0.9993181,0.00005123182,0.0003147366,0.000081568025,0.0001211779,0.00011318055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037422084,0.00038920814,0.00034284897,0.0011954563,0.00045494668,0.00047890312,0.00032722065,0.00028715536,0.0014067447],"category_scores_gemma":[0.00065097475,0.00014182809,0.0002904512,0.0009990799,0.0001682419,0.0003362478,0.00090323034,0.00033897458,0.0008100688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024975796,0.00008817093,0.9519834,0.0000718814,0.00015239061,0.00058436685,0.00036319508,0.00046117732,0.010255634,0.00012811078,0.0015095696,0.034152456],"study_design_scores_gemma":[0.000005118338,0.00013600143,0.98947036,0.000011241667,0.00003708525,0.0005617723,0.000080925965,0.00020557843,0.0013175157,0.00003617487,0.008130533,0.0000076179044],"about_ca_topic_score_codex":0.004654323,"about_ca_topic_score_gemma":0.008555466,"teacher_disagreement_score":0.004654323,"about_ca_system_score_codex":0.00029001868,"about_ca_system_score_gemma":0.00019227277,"threshold_uncertainty_score":0.009254456},"labels":[],"label_agreement":null},{"id":"W2000077629","doi":"10.1086/427978","title":"The Disk and Extraplanar Regions of NGC 55","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Red supergiant; Star formation; Stars; Astronomy; Asymptotic giant branch; Hubble sequence; Stellar population; Spiral galaxy; Supergiant","score_opus":0.006828693705088632,"score_gpt":0.20806904256120753,"score_spread":0.2012403488561189,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000077629","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982274,0.00021127533,0.000064655025,0.000007210509,0.000001392362,7.840684e-7,0.000101326266,0.000009340564,0.0013765167],"genre_scores_gemma":[0.9992861,0.00008916954,0.00010547298,0.0000059618064,0.0000018202956,5.388343e-7,0.00023178455,0.0000018144859,0.00027738838],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999566,0.0000020504099,0.0000024575231,0.000016529653,0.000007784374,0.000014506088],"domain_scores_gemma":[0.9998895,0.000008162987,0.000046801382,0.0000112163925,0.000011347525,0.00003292546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005271598,0.00016775525,0.00007575428,0.00066268165,0.00020388079,0.00033850037,0.00011086154,0.00010038627,0.0012874888],"category_scores_gemma":[0.00019002627,0.00009217285,0.00011611537,0.00031362422,0.00019650203,0.00016741584,0.00026436764,0.00006736741,0.0002856835],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004035525,0.000038219056,0.7342523,0.00009928634,0.00008605589,0.0015882642,0.0015725824,0.0009662158,0.23290458,0.0016207942,0.00066078,0.025807476],"study_design_scores_gemma":[0.0000027888966,0.000029934152,0.995282,0.000007675901,0.000017008957,0.00050344114,0.00015057444,0.00025449146,0.0016483391,0.00005315738,0.0020477155,0.0000028466866],"about_ca_topic_score_codex":0.01639731,"about_ca_topic_score_gemma":0.014594815,"teacher_disagreement_score":0.01639731,"about_ca_system_score_codex":0.00043688482,"about_ca_system_score_gemma":0.00009458195,"threshold_uncertainty_score":0.03260368},"labels":[],"label_agreement":null},{"id":"W2000144197","doi":"10.1088/0004-637x/734/1/54","title":"THE RADIO-2 mm SPECTRAL INDEX OF THE CRAB NEBULA MEASURED WITH GISMO","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Crab Nebula; Spectral index; Flattening; Millimeter; Bolometer; Nebula; Supernova remnant; Synchrotron; Submillimeter Array; Spectral resolution","score_opus":0.016795957650757507,"score_gpt":0.2012810684562107,"score_spread":0.18448511080545318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000144197","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99204034,0.00027046545,0.0013473242,0.00003854851,0.0000094680945,0.0000088960805,0.0013055371,0.00014022212,0.004839267],"genre_scores_gemma":[0.9952077,0.00014417198,0.001968001,0.000039395676,0.000017339991,0.00002043501,0.0017562889,0.000031863696,0.0008148216],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991643,0.0000071370987,0.0000032991647,0.000025978343,0.000026864223,0.000020275684],"domain_scores_gemma":[0.9997905,0.000029679093,0.0000757601,0.000023916695,0.000040755433,0.000039373117],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013606202,0.0002215887,0.00015756451,0.0010552397,0.00016668854,0.00031893834,0.00023116282,0.00026756903,0.0014463245],"category_scores_gemma":[0.00034314833,0.00017190282,0.00015050339,0.0006714045,0.00011742089,0.00019852348,0.00029935024,0.00020546031,0.00046818255],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000492455,0.000075449294,0.41736552,0.00013765854,0.00011673262,0.00054595876,0.00051642885,0.0011162467,0.5595128,0.0006145927,0.0013696525,0.01813647],"study_design_scores_gemma":[0.000007051559,0.000046737954,0.984411,0.0000068997415,0.000019083564,0.00023452677,0.000050435247,0.0006480317,0.012266401,0.000067006076,0.0022329106,0.000009833838],"about_ca_topic_score_codex":0.0011569286,"about_ca_topic_score_gemma":0.0029506735,"teacher_disagreement_score":0.0014463245,"about_ca_system_score_codex":0.00019519671,"about_ca_system_score_gemma":0.00007774282,"threshold_uncertainty_score":0.0048384666},"labels":[],"label_agreement":null},{"id":"W2000153388","doi":"10.1088/0004-637x/714/1/194","title":"UNSTABLE PLANETARY SYSTEMS EMERGING OUT OF GAS DISKS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph","funders":"","keywords":"Planet; Planetary system; Physics; Exoplanet; Eccentricity (behavior); Planetary migration; Gas giant; Astrophysics; Dissipation; Solar System; Planetary mass; Debris disk; Protoplanetary disk","score_opus":0.01061694495812279,"score_gpt":0.22532348039598546,"score_spread":0.21470653543786267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000153388","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900711,0.00010587969,0.0064658457,0.000073867035,0.0000110965775,0.000018848106,0.00006293694,0.00008117799,0.003109223],"genre_scores_gemma":[0.99703026,0.000061547966,0.0023058818,0.000024395948,0.0000044510894,0.00001539636,0.000052435476,0.000019294754,0.00048638886],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993694,0.000014265596,0.0000033579895,0.000012961651,0.00001584715,0.00001662166],"domain_scores_gemma":[0.99972874,0.000088317065,0.000070380214,0.000030078789,0.000026943226,0.000055492612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014631418,0.00026439183,0.00032289824,0.00027616395,0.0006008704,0.00066670583,0.00046178233,0.00055681757,0.0009594635],"category_scores_gemma":[0.0011124086,0.0002564344,0.00041121276,0.00023877791,0.0007359472,0.00056381745,0.0007555834,0.00041200715,0.00010291873],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013098588,0.00010048381,0.035173275,0.0000911845,0.00008993371,0.0012032837,0.00056869193,0.91683906,0.023357473,0.014893535,0.0005777522,0.006974328],"study_design_scores_gemma":[0.000059728798,0.00007066644,0.009347296,0.000014184533,0.0000217157,0.00021579351,0.00017770339,0.98214114,0.0027642848,0.0043007773,0.0008700519,0.000016726763],"about_ca_topic_score_codex":0.0048911027,"about_ca_topic_score_gemma":0.0029148061,"teacher_disagreement_score":0.0048911027,"about_ca_system_score_codex":0.00062632817,"about_ca_system_score_gemma":0.00044010693,"threshold_uncertainty_score":0.009725273},"labels":[],"label_agreement":null},{"id":"W2000158638","doi":"10.1088/0004-637x/691/2/946","title":"THE SIZES AND LUMINOSITIES OF MASSIVE STAR CLUSTERS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Solar mass; Star cluster; Cluster (spacecraft); Dark matter; Milky Way; Stellar mass; Galaxy cluster; Mass segregation; RADIUS","score_opus":0.007612854702407951,"score_gpt":0.2501522483601701,"score_spread":0.24253939365776214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000158638","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9891138,0.0012104851,0.0004920458,0.00007899329,0.000012619403,0.0000076190177,0.00088478584,0.000051838968,0.008147859],"genre_scores_gemma":[0.9963731,0.00048085212,0.00050966896,0.000030143616,0.000031635944,0.000010098474,0.0012899061,0.000014551916,0.0012600158],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997365,0.000021114107,0.000020798323,0.000106098305,0.000068070774,0.000047440688],"domain_scores_gemma":[0.9989579,0.00026098077,0.0003987718,0.00008504507,0.000120013676,0.00017728093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032392528,0.00014255427,0.0001632703,0.0017536258,0.0005810523,0.001121593,0.00030839248,0.00020474494,0.002124947],"category_scores_gemma":[0.0022924915,0.00021603674,0.00018491711,0.00093569956,0.00039215558,0.00046348086,0.00089351495,0.0002540561,0.00052045524],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001366752,0.00002262686,0.9487842,0.00008127764,0.00009712671,0.00015602219,0.0016580092,0.0018867357,0.0117645785,0.0062968913,0.002090666,0.027025286],"study_design_scores_gemma":[0.00000369355,0.000020330013,0.99244434,0.00001467008,0.000012784371,0.00025102,0.00027045538,0.00049983215,0.0012463873,0.0010931685,0.004133508,0.000009884556],"about_ca_topic_score_codex":0.0021227077,"about_ca_topic_score_gemma":0.0017977315,"teacher_disagreement_score":0.002124947,"about_ca_system_score_codex":0.000558142,"about_ca_system_score_gemma":0.0001716185,"threshold_uncertainty_score":0.0071086287},"labels":[],"label_agreement":null},{"id":"W2000175712","doi":"10.1088/0004-637x/714/1/713","title":"THE NGC 404 NUCLEUS: STAR CLUSTER AND POSSIBLE INTERMEDIATE-MASS BLACK HOLE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":172,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Star cluster; Black hole (networking); Intermediate-mass black hole; Surface brightness; Stellar mass; Galaxy; Stellar black hole; Stellar kinematics; Bulge","score_opus":0.004541165624043316,"score_gpt":0.20526644837315777,"score_spread":0.20072528274911447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000175712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99924964,0.000042697382,0.0000810502,0.00000808843,0.0000011050001,0.0000016097464,0.00005765238,0.000009891201,0.0005482887],"genre_scores_gemma":[0.99916375,0.000027638785,0.00023662686,0.000006429725,0.0000023391333,0.000002323364,0.00017642416,0.0000029719336,0.00038151603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999448,0.0000044041094,0.0000020987811,0.000017819404,0.000011580101,0.000019235846],"domain_scores_gemma":[0.9998909,0.0000068681284,0.00004264646,0.000009526671,0.000011198068,0.00003875162],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010340034,0.00033097022,0.00018814513,0.00083924434,0.00053247384,0.0003239225,0.0003331333,0.00032985857,0.0014545337],"category_scores_gemma":[0.00014656357,0.00012193064,0.00016280361,0.0005016685,0.00038244098,0.00025411256,0.0004096598,0.000085872074,0.00042275703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004980684,0.000077031145,0.88448405,0.00004673539,0.000047445337,0.003418212,0.00076579396,0.0011821189,0.10162497,0.0006015649,0.00043734192,0.0068166624],"study_design_scores_gemma":[0.0000126366185,0.00018217508,0.98797834,0.000008050637,0.000021651274,0.0023404886,0.0006005755,0.00207815,0.004280809,0.00054872263,0.0019347657,0.000013759239],"about_ca_topic_score_codex":0.009725555,"about_ca_topic_score_gemma":0.013789333,"teacher_disagreement_score":0.009725555,"about_ca_system_score_codex":0.0005240586,"about_ca_system_score_gemma":0.00018279575,"threshold_uncertainty_score":0.019337893},"labels":[],"label_agreement":null},{"id":"W2000237959","doi":"10.1086/426380","title":"Radial Velocity Detectability of Low‐Mass Extrasolar Planets in Close Orbits","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Planet; Radial velocity; Jupiter mass; Astrophysics; Minimum mass; Exoplanet; Astronomy; Planetary migration; Protoplanetary disk; Planetary mass; Giant planet; Orbital speed; Hot Jupiter; Planetary system; Stars","score_opus":0.008039491024511833,"score_gpt":0.21923269745058924,"score_spread":0.21119320642607742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000237959","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99717593,0.00013946983,0.0015005628,0.00003194145,0.000003634142,0.0000032648459,0.000079602076,0.00002712905,0.0010383722],"genre_scores_gemma":[0.9995003,0.00002113333,0.00022629605,0.000005956139,0.000005334376,0.0000013502615,0.00013020073,0.0000033629824,0.00010600902],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.998906,0.00030219337,0.00008960985,0.00033647596,0.00023114111,0.00013455637],"domain_scores_gemma":[0.97636706,0.01419183,0.0049999333,0.0017996102,0.0015851514,0.0010563463],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019464515,0.00020199073,0.00041189068,0.0014907526,0.0003539852,0.0008867989,0.00041808008,0.0007811494,0.0015902725],"category_scores_gemma":[0.016513426,0.00017433958,0.00020670649,0.0005299404,0.0006706972,0.0007285689,0.00078399107,0.00036174626,0.00035134229],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023050883,0.000032408752,0.97417986,0.000025831858,0.000045885172,0.00013551537,0.00018172599,0.0014576417,0.00977627,0.00096095185,0.00019799412,0.012775368],"study_design_scores_gemma":[0.000013052134,0.00025698086,0.9714211,0.00001704405,0.00006163731,0.0018623669,0.00020505994,0.01266285,0.010361928,0.002257041,0.0008505713,0.000030404017],"about_ca_topic_score_codex":0.0006668466,"about_ca_topic_score_gemma":0.000756488,"teacher_disagreement_score":0.0019464515,"about_ca_system_score_codex":0.00026371234,"about_ca_system_score_gemma":0.00013667539,"threshold_uncertainty_score":0.010293901},"labels":[],"label_agreement":null},{"id":"W2000307147","doi":"10.1086/498560","title":"The Discordance of Mass‐Loss Estimates for Galactic O‐Type Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":389,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Stars; Astrophysics; Physics; Ion; Estimator; Statistics","score_opus":0.009239030137668672,"score_gpt":0.23627017974503228,"score_spread":0.22703114960736362,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000307147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973418,0.00015512275,0.0018293135,0.000009522233,0.0000029851801,0.000004746036,0.00018986437,0.00002976937,0.00043692565],"genre_scores_gemma":[0.99888474,0.000071148424,0.00057561736,0.0000069387324,0.0000026554765,0.0000032458843,0.00035538763,0.000011667996,0.00008859143],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995546,0.000068093905,0.000057439003,0.00015550014,0.000104154715,0.0000602511],"domain_scores_gemma":[0.9985807,0.00043770796,0.0004414621,0.00024668738,0.00022229989,0.000071170674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010154819,0.00064844557,0.00036531617,0.001333953,0.00030862863,0.00090481096,0.00056518463,0.0004001517,0.00035641837],"category_scores_gemma":[0.0034924918,0.00027949963,0.00037690872,0.0004682522,0.00030083882,0.0004831591,0.00071340095,0.00022429017,0.00029301643],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032175364,0.000014934825,0.9632674,0.00003321225,0.00018470397,0.000094497016,0.00023530883,0.004793928,0.019913083,0.00024696472,0.00007874294,0.010815561],"study_design_scores_gemma":[0.000019047033,0.00007972069,0.97120756,0.000011549139,0.000058788344,0.00030741232,0.00014960534,0.0128904935,0.0138833085,0.000543814,0.00082881097,0.000019817078],"about_ca_topic_score_codex":0.002538823,"about_ca_topic_score_gemma":0.002732848,"teacher_disagreement_score":0.002538823,"about_ca_system_score_codex":0.00039530735,"about_ca_system_score_gemma":0.00008811316,"threshold_uncertainty_score":0.005370438},"labels":[],"label_agreement":null},{"id":"W2000338645","doi":"10.1086/426536","title":"Simulating the<i>Spitzer</i>Mid‐Infrared Color‐Color Diagrams","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Galaxy; Astrophysics; Physics; Redshift; Infrared; Astronomy","score_opus":0.007853088912844216,"score_gpt":0.21890664805222412,"score_spread":0.2110535591393799,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000338645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.938643,0.000056465302,0.05440404,0.00025780144,0.000026132071,0.00006393215,0.0010488302,0.00047817416,0.005021673],"genre_scores_gemma":[0.98431075,0.000034680706,0.013714446,0.00004543913,0.000006684457,0.00007298024,0.00061572995,0.000053515934,0.0011458471],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998381,0.000055542365,0.0000056252493,0.000035860572,0.00001933594,0.00004555594],"domain_scores_gemma":[0.99776185,0.0014681057,0.0002005242,0.0001669907,0.00023347492,0.00016906779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071672193,0.00031434806,0.00041188832,0.0007523165,0.00049809867,0.0007657854,0.0012358469,0.0012239546,0.003704612],"category_scores_gemma":[0.0037321898,0.000502167,0.00061919744,0.000737151,0.00064517773,0.00083144504,0.0005366972,0.00079957943,0.0003475949],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034291366,0.000021526874,0.005315009,0.0000073612,0.000009639688,0.000030680796,0.000034694385,0.9895104,0.00033358444,0.0034298773,0.00018940243,0.0010836952],"study_design_scores_gemma":[0.000013573649,0.0000065215954,0.00083829643,0.0000019418699,0.0000036983224,0.000006538198,0.000010575695,0.997615,0.0002139082,0.0011475995,0.00013714365,0.000005185129],"about_ca_topic_score_codex":0.039901942,"about_ca_topic_score_gemma":0.028960569,"teacher_disagreement_score":0.039901942,"about_ca_system_score_codex":0.0016383453,"about_ca_system_score_gemma":0.00095978205,"threshold_uncertainty_score":0.079339385},"labels":[],"label_agreement":null},{"id":"W2000410790","doi":"10.1086/508858","title":"Evidence against Macroscopic Astrophysical Dyadospheres","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Space Technology and Applications","field":"Engineering","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Pair production; Electric field; Production (economics); Electron; Field (mathematics); Wavelength; Compton scattering; Production rate","score_opus":0.009084979180470793,"score_gpt":0.22756248268249968,"score_spread":0.21847750350202888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000410790","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92459273,0.0028255335,0.00846339,0.0020157532,0.00012003816,0.000019545038,0.0002514125,0.00022166458,0.06149004],"genre_scores_gemma":[0.9975152,0.00055498607,0.00061989506,0.00012397309,0.0000231941,0.000005670888,0.00010169661,0.000011955434,0.0010434305],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998217,0.000020977515,0.000007092863,0.00004730747,0.00006356088,0.00003932789],"domain_scores_gemma":[0.99865484,0.00043291363,0.00025571187,0.00028252086,0.00013907046,0.00023490118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003161161,0.00018096338,0.00025100028,0.0004358752,0.0004958402,0.0010432587,0.0003520113,0.0005262523,0.004170979],"category_scores_gemma":[0.0014682855,0.00017529938,0.00013995174,0.00028600317,0.002080226,0.0008707419,0.0016901683,0.00073597743,0.0005603974],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024472014,0.0001384853,0.20174834,0.0011787757,0.00028593474,0.008689222,0.0026753147,0.004339581,0.2926847,0.4052781,0.009083116,0.0714513],"study_design_scores_gemma":[0.00037267382,0.0011663185,0.4216602,0.00021938262,0.00022855049,0.025288707,0.0040836227,0.007399209,0.13015991,0.24359365,0.16566512,0.00016267449],"about_ca_topic_score_codex":0.00044895604,"about_ca_topic_score_gemma":0.0005044494,"teacher_disagreement_score":0.004170979,"about_ca_system_score_codex":0.00026011054,"about_ca_system_score_gemma":0.00015562921,"threshold_uncertainty_score":0.013953328},"labels":[],"label_agreement":null},{"id":"W2000412191","doi":"10.1086/308192","title":"The<i>Hubble Space Telescope</i>Key Project on the Extragalactic Distance Scale. XXI. The Cepheid Distance to NGC 1425","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Distance modulus; Physics; Cosmic distance ladder; Astrophysics; Photometry (optics); Astronomy; Large Magellanic Cloud; Hubble space telescope; Hubble's law; Extinction (optical mineralogy); Galaxy; Stars; Redshift","score_opus":0.009433739551890226,"score_gpt":0.2260477893536991,"score_spread":0.21661404980180887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000412191","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.062261865,0.016284533,0.018032886,0.0037895157,0.0026001737,0.0005112073,0.57111686,0.0042932853,0.3211097],"genre_scores_gemma":[0.20781314,0.0068934085,0.044611726,0.0007152813,0.00083900214,0.00051512284,0.6078106,0.00074088183,0.1300608],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99967194,0.000036795795,0.000014062551,0.00006160849,0.00015996129,0.00005572401],"domain_scores_gemma":[0.99911076,0.00004818747,0.00026677933,0.00012687889,0.0002316133,0.00021567167],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006934191,0.00091623905,0.00033892112,0.0025666212,0.0005035767,0.0009286268,0.0005520626,0.00033163695,0.036835954],"category_scores_gemma":[0.001046283,0.00017312072,0.00019510777,0.0031478114,0.00020330248,0.0008158028,0.00091233855,0.0006997502,0.015804145],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003045838,0.00007203286,0.031995744,0.0004166281,0.000046019322,0.000117050506,0.00021931865,0.00022072408,0.0035933147,0.023305982,0.6825798,0.25712878],"study_design_scores_gemma":[0.00004040488,0.000039546518,0.2251115,0.000061701576,0.0000113105325,0.00010880973,0.000052665247,0.0003268945,0.0008214459,0.0038474519,0.7695646,0.0000135754735],"about_ca_topic_score_codex":0.019636136,"about_ca_topic_score_gemma":0.01581721,"teacher_disagreement_score":0.036835954,"about_ca_system_score_codex":0.0012573627,"about_ca_system_score_gemma":0.0007558103,"threshold_uncertainty_score":0.12322849},"labels":[],"label_agreement":null},{"id":"W2000627331","doi":"10.1088/0004-637x/692/2/1561","title":"<i>SPITZER</i>OBSERVATIONS OF EXTENDED LYMAN-α CLOUDS IN THE SSA22 FIELD","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Astronomy; QSOS; Halo; Population; Active galactic nucleus; Quasar","score_opus":0.012199704346904764,"score_gpt":0.23165238684567085,"score_spread":0.2194526824987661,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000627331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99874914,0.00007362494,0.000067630055,0.000011668714,8.9395877e-7,0.0000019156412,0.00022867654,0.000013173462,0.00085313374],"genre_scores_gemma":[0.9986382,0.00010287388,0.00028777277,0.00001334991,0.000013095458,0.0000030665753,0.00063212035,0.0000033800275,0.00030622998],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999443,0.0000044439394,0.0000026098674,0.000010460229,0.000012977221,0.000025117035],"domain_scores_gemma":[0.9997526,0.00001180427,0.00009504932,0.000024290182,0.000030126273,0.00008608588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011641916,0.00026337942,0.00017829034,0.0015819737,0.00030237233,0.00043491417,0.00014495634,0.00013079424,0.0011482079],"category_scores_gemma":[0.00019872122,0.00010615815,0.00012755918,0.000912669,0.00020643724,0.0002450604,0.00032036912,0.000121772624,0.00023182608],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025307047,0.0001043017,0.908347,0.00004478924,0.00008768488,0.0006882088,0.00066424237,0.0013024696,0.07067727,0.00030119196,0.0011862741,0.016343635],"study_design_scores_gemma":[0.000007577272,0.00004266142,0.9972709,0.0000043674254,0.000015366873,0.00017404622,0.000101242396,0.0003352507,0.0009818451,0.000049411203,0.0010129141,0.000004316354],"about_ca_topic_score_codex":0.013100209,"about_ca_topic_score_gemma":0.02537555,"teacher_disagreement_score":0.013100209,"about_ca_system_score_codex":0.00029708337,"about_ca_system_score_gemma":0.00012082003,"threshold_uncertainty_score":0.026047885},"labels":[],"label_agreement":null},{"id":"W2000643541","doi":"10.1088/0004-637x/784/1/52","title":"HerMES: SPECTRAL ENERGY DISTRIBUTIONS OF SUBMILLIMETER GALAXIES AT<i>z</i>&gt; 4","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Luminosity; Luminous infrared galaxy; Spectral index; Infrared; Spectral energy distribution; Sample (material); Radio galaxy; Extinction (optical mineralogy)","score_opus":0.005277000431082794,"score_gpt":0.19182129373890336,"score_spread":0.18654429330782057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000643541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959157,0.0000484017,0.00030086725,0.000024267145,0.0000021620203,0.000005510092,0.0024357734,0.00007407286,0.001193252],"genre_scores_gemma":[0.99201804,0.000043589152,0.0005036088,0.000016374766,0.000011088219,0.00000985759,0.00638881,0.000023107366,0.0009853903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999866,0.000013245482,0.000006711421,0.00004033067,0.000037677168,0.0000360424],"domain_scores_gemma":[0.9993463,0.00009967191,0.0002600282,0.000076866534,0.00007281125,0.00014426322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034575272,0.000250001,0.00018471233,0.0017401585,0.00015975175,0.0004999571,0.0002696354,0.00011897547,0.0022884684],"category_scores_gemma":[0.00063746516,0.00010933579,0.0002510831,0.0008242119,0.00016728499,0.00028214324,0.00039761927,0.00017642355,0.0006482954],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012613813,0.00003036258,0.9807016,0.000013611893,0.000055276996,0.00008100998,0.0003591207,0.00048299215,0.004635354,0.00042616023,0.0012944242,0.011793933],"study_design_scores_gemma":[0.0000029998391,0.000017986837,0.9977791,0.0000011446301,0.000006819309,0.000057566434,0.00007942857,0.00043711058,0.00045666378,0.00005773407,0.0011006012,0.0000028916575],"about_ca_topic_score_codex":0.0035085932,"about_ca_topic_score_gemma":0.005274189,"teacher_disagreement_score":0.0035085932,"about_ca_system_score_codex":0.0002743665,"about_ca_system_score_gemma":0.00006899092,"threshold_uncertainty_score":0.00765568},"labels":[],"label_agreement":null},{"id":"W2000651916","doi":"10.1088/0004-637x/768/1/64","title":"THE CORRELATION BETWEEN DISPERSION MEASURE AND X-RAY COLUMN DENSITY FROM RADIO PULSARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":139,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Ionization; Dispersion (optics); Electron density; Interstellar medium; Line (geometry); Observatory; Measure (data warehouse); Extinction (optical mineralogy)","score_opus":0.009364130955708011,"score_gpt":0.2599455831860419,"score_spread":0.2505814522303339,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000651916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998268,0.000222039,0.0004197353,0.000012575899,0.0000025126071,0.0000015938815,0.00014681874,0.0000135418695,0.00091315876],"genre_scores_gemma":[0.9993131,0.00008564515,0.00017002647,0.0000047002836,0.000007594404,0.0000024306182,0.0002564851,0.0000024594292,0.00015759227],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980694,0.000034541987,0.000023587238,0.000047701178,0.000060817292,0.00002641706],"domain_scores_gemma":[0.996743,0.001731645,0.00090890063,0.0002603073,0.00022226865,0.00013389112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002798316,0.00020467097,0.00016800944,0.0014265996,0.00019463786,0.00042759272,0.0001808911,0.00024686495,0.0011559437],"category_scores_gemma":[0.0029623641,0.00010897981,0.00010973155,0.00083812315,0.00024491138,0.00038056038,0.0004306322,0.00020574378,0.00028894757],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030009594,0.000010643247,0.99298614,0.000010464796,0.000035340054,0.000034034787,0.00007245681,0.0003028605,0.0023966215,0.0000856285,0.000046285626,0.0039895987],"study_design_scores_gemma":[8.395996e-7,0.000020352772,0.9982168,0.0000031975387,0.000007789729,0.00018327439,0.00005222463,0.0004992725,0.0007570358,0.00007429118,0.00018146008,0.000003444013],"about_ca_topic_score_codex":0.00083776744,"about_ca_topic_score_gemma":0.0010286073,"teacher_disagreement_score":0.0014265996,"about_ca_system_score_codex":0.00011353376,"about_ca_system_score_gemma":0.00006122298,"threshold_uncertainty_score":0.0038670301},"labels":[],"label_agreement":null},{"id":"W2000771032","doi":"10.1086/342877","title":"Revised Stellar Temperatures for Magellanic Cloud O Supergiants from<i>Far Ultraviolet Spectroscopic Explorer</i>and Very Large Telescope UV‐Visual Echelle Spectrograph Spectroscopy","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":211,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supergiant; Blanketing; Physics; Astrophysics; Microturbulence; Spectrograph; Astronomy; Ultraviolet; Small Magellanic Cloud; Red supergiant; Stellar atmosphere; Large Magellanic Cloud; Spectroscopy; Stars; Space Telescope Imaging Spectrograph; Spectral line; Hubble space telescope; Optics","score_opus":0.011740936608893346,"score_gpt":0.2355155196721924,"score_spread":0.22377458306329906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000771032","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9710154,0.0006819798,0.008106272,0.00010115938,0.00008554041,0.000059841906,0.010728692,0.00029154844,0.008929571],"genre_scores_gemma":[0.9684529,0.00032616837,0.0114744725,0.00008190325,0.00003013357,0.0000726757,0.017247118,0.00014845267,0.0021661168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997702,0.000020938658,0.000024024612,0.0000679168,0.00007792694,0.00003896546],"domain_scores_gemma":[0.9992762,0.00006247659,0.00020971277,0.0000888888,0.00029111237,0.00007167089],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006733525,0.00037413964,0.00023055902,0.0011273425,0.0003523247,0.0005908951,0.00055658596,0.00026546052,0.001547058],"category_scores_gemma":[0.0011065577,0.00014701343,0.00045056932,0.0006900991,0.00012605787,0.000505059,0.00039532845,0.00039178735,0.0010697341],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032041807,0.000043577747,0.89670825,0.00030298726,0.00016124391,0.00020239488,0.00097546715,0.004097393,0.04347831,0.0011674545,0.004190276,0.04835219],"study_design_scores_gemma":[0.000011389842,0.00006264324,0.9815004,0.000023299204,0.00004103991,0.00013001438,0.00019987804,0.0018596457,0.0056185955,0.0002677226,0.010271251,0.000014072506],"about_ca_topic_score_codex":0.0072977706,"about_ca_topic_score_gemma":0.01444152,"teacher_disagreement_score":0.0072977706,"about_ca_system_score_codex":0.00065767276,"about_ca_system_score_gemma":0.00025670498,"threshold_uncertainty_score":0.014510632},"labels":[],"label_agreement":null},{"id":"W2000778101","doi":"10.1088/0004-637x/702/1/824","title":"ERRATUM: “LYMAN α RADIATIVE TRANSFER IN COSMOLOGICAL SIMULATIONS USING ADAPTIVE MESH REFINEMENT” (2009, ApJ, 696, 853)","year":2009,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Advanced Thermodynamics and Statistical Mechanics","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Radiative transfer; Gaussian; Astrophysics; Function (biology); Acceleration; Core (optical fiber); Statistical physics; Computational physics; Applied mathematics; Classical mechanics; Quantum mechanics; Optics; Mathematics","score_opus":0.02180237677678659,"score_gpt":0.2774778144077324,"score_spread":0.2556754376309458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000778101","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011204311,0.0017884932,0.0018487027,0.038742173,0.9380317,0.000049551752,0.00458051,0.0011330385,0.012705529],"genre_scores_gemma":[0.037444625,0.008552022,0.014734257,0.05940663,0.10775698,0.00028190968,0.02335177,0.007759792,0.7407119],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99852353,0.0001774149,0.0002485065,0.00022310718,0.0007334466,0.00009391895],"domain_scores_gemma":[0.99451643,0.0013027809,0.00035460587,0.00045338066,0.0030553024,0.00031745643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018547615,0.0018944858,0.0014988362,0.002048011,0.0031598737,0.00330662,0.0028700419,0.0031222769,0.0744819],"category_scores_gemma":[0.020590287,0.0008435638,0.0011419746,0.0019750032,0.0011746712,0.0031951654,0.0017902061,0.0050040646,0.03944815],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046570065,0.000010622066,0.00009392431,0.00005679255,0.000008545348,0.00011283221,0.000014985757,0.00012301213,0.00010118941,0.0008210069,0.99480325,0.0038073123],"study_design_scores_gemma":[0.00008553144,0.000050495277,0.0026759633,0.0003133962,0.00004996638,0.00046578515,0.00014915653,0.0018506208,0.0017571518,0.00416033,0.98834246,0.00009921896],"about_ca_topic_score_codex":0.014892107,"about_ca_topic_score_gemma":0.021914905,"teacher_disagreement_score":0.0744819,"about_ca_system_score_codex":0.0027477266,"about_ca_system_score_gemma":0.0024821197,"threshold_uncertainty_score":0.24916679},"labels":[],"label_agreement":null},{"id":"W2000794423","doi":"10.1088/0004-637x/760/2/131","title":"THE DEPENDENCE OF QUENCHING UPON THE INNER STRUCTURE OF GALAXIES AT 0.5 ⩽<i>z</i>&lt; 0.8 IN THE DEEP2/AEGIS SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":245,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Galaxy; Quenching (fluorescence); Stellar mass; Star formation; Stellar population; Redshift; Population; Galaxy formation and evolution","score_opus":0.009352014726271103,"score_gpt":0.22155095606851102,"score_spread":0.21219894134223993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000794423","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99870574,0.00006788526,0.00012208433,0.000041174808,0.0000012537604,0.0000017047921,0.0002583813,0.000016773369,0.0007849455],"genre_scores_gemma":[0.9994941,0.000020580825,0.000038669765,0.000008554004,0.0000028313063,0.000001088821,0.00030015418,0.000002923821,0.00013108512],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996798,0.000041858537,0.00001834073,0.00010230349,0.00006135322,0.0000962812],"domain_scores_gemma":[0.99718,0.0004984138,0.0011627971,0.0003025976,0.00031959944,0.0005365545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003991638,0.00014015926,0.00016498394,0.0009454992,0.00024583968,0.00056621316,0.0003223148,0.00027376448,0.0013540694],"category_scores_gemma":[0.0020899086,0.00014088444,0.00021593191,0.0005156949,0.0005736065,0.0004295216,0.00068286853,0.00028909056,0.00038415712],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003179392,0.00000530291,0.99668497,0.0000029349476,0.000013624903,0.0000140571365,0.00012214991,0.00009260808,0.0011801248,0.00009521314,0.000101306985,0.0016558665],"study_design_scores_gemma":[2.9843946e-7,0.000004947767,0.9997193,5.343986e-7,0.0000017290638,0.000012305899,0.000028780434,0.00007240045,0.00007840617,0.000015147865,0.00006553411,6.517119e-7],"about_ca_topic_score_codex":0.009322102,"about_ca_topic_score_gemma":0.014065036,"teacher_disagreement_score":0.009322102,"about_ca_system_score_codex":0.0003163292,"about_ca_system_score_gemma":0.00010600308,"threshold_uncertainty_score":0.018535674},"labels":[],"label_agreement":null},{"id":"W2000821703","doi":"10.1086/422897","title":"Relationship between Environment and the Broadband Optical Properties of Galaxies in the Sloan Digital Sky Survey","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":621,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Astrophysics; Sky; Galaxy; Physics; Luminosity; Surface brightness; Astronomy; Surface brightness fluctuation; Luminous infrared galaxy; Brightest cluster galaxy","score_opus":0.018850051182921247,"score_gpt":0.20666536708859443,"score_spread":0.18781531590567319,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000821703","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99928576,0.00006187516,0.00004640484,0.0000350725,9.135925e-7,5.4039333e-7,0.00026470944,0.0000031755862,0.00030153632],"genre_scores_gemma":[0.9993888,0.00003935287,0.0000288358,0.000006464619,0.000002722146,6.6832087e-7,0.00039107536,0.0000016934008,0.00014034341],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997514,0.000079759426,0.000021593152,0.00005194165,0.000036566504,0.00005869672],"domain_scores_gemma":[0.9962174,0.0010768785,0.0015512946,0.00024636093,0.0003622912,0.00054566684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005524955,0.00014619522,0.00013880491,0.00087929453,0.00025809524,0.0006204767,0.00014718567,0.0001975209,0.0014280037],"category_scores_gemma":[0.0028250862,0.00012999686,0.00020018211,0.00092982996,0.0003981087,0.00045719848,0.0006681656,0.0002685289,0.0002420996],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000015042315,0.0000052736405,0.99908924,0.000001325767,0.000025128873,0.000011701422,0.000028512839,0.0001403605,0.000088715686,0.000031798903,0.000039125112,0.0005237696],"study_design_scores_gemma":[4.3617305e-7,0.0000046600035,0.9997528,5.337961e-7,0.0000042406027,0.000011444607,0.00003146284,0.00010972712,0.000015789175,0.000019871602,0.00004801671,8.933419e-7],"about_ca_topic_score_codex":0.01475783,"about_ca_topic_score_gemma":0.025898244,"teacher_disagreement_score":0.01475783,"about_ca_system_score_codex":0.0003219137,"about_ca_system_score_gemma":0.00020157131,"threshold_uncertainty_score":0.029343903},"labels":[],"label_agreement":null},{"id":"W2000972033","doi":"10.1086/375486","title":"Cluster Sunyaev‐Zeldovich Effect Scaling Relations","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Intracluster medium; Astrophysics; Redshift; Galaxy cluster; Scaling; Observable; Cluster (spacecraft); Entropy (arrow of time); Galaxy; Sunyaev–Zel'dovich effect; Statistical physics; Thermodynamics; Quantum mechanics; Geometry","score_opus":0.005189834913264445,"score_gpt":0.2123980781645658,"score_spread":0.20720824325130136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2000972033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9832161,0.0004952495,0.0082917055,0.00008914082,0.000013671869,0.000016603592,0.00023010392,0.00018044449,0.0074669695],"genre_scores_gemma":[0.99920803,0.00006805744,0.00045790107,0.000005413347,0.00001310148,0.000005702832,0.00006435688,0.000007316934,0.00017016593],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984026,0.000025374307,0.000010612515,0.000039092025,0.000048412916,0.00003620894],"domain_scores_gemma":[0.99798715,0.0007762082,0.0005245943,0.0003282885,0.0001576262,0.00022619085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036478078,0.0002383105,0.0002973843,0.0008074901,0.00028428098,0.00051295245,0.0002268549,0.00011104247,0.0017121172],"category_scores_gemma":[0.0027942492,0.0001366359,0.00022923858,0.0003134293,0.00060621696,0.00034464448,0.000547875,0.00023969737,0.00015834229],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052816875,0.00008137514,0.5382664,0.00023445082,0.0003381215,0.0011495356,0.0014661949,0.11373767,0.032523558,0.26398936,0.0037545597,0.04393053],"study_design_scores_gemma":[0.00007042365,0.00013047937,0.6284073,0.00004260117,0.0001138932,0.001062633,0.0001934811,0.19083045,0.008314581,0.16603576,0.004675935,0.00012243404],"about_ca_topic_score_codex":0.001254438,"about_ca_topic_score_gemma":0.0005294648,"teacher_disagreement_score":0.0017121172,"about_ca_system_score_codex":0.00037756178,"about_ca_system_score_gemma":0.00020088804,"threshold_uncertainty_score":0.005727589},"labels":[],"label_agreement":null},{"id":"W2001032132","doi":"10.1086/509871","title":"Velocity Distributions from Nonextensive Thermodynamics","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Statistical Mechanics and Entropy","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Polytropic process; Physics; Statistical physics; Work (physics); Monotonic function; Dark matter; Distribution (mathematics); Thermodynamics; Theoretical physics; Classical mechanics; Mathematics; Astrophysics; Mathematical analysis","score_opus":0.008610738008851482,"score_gpt":0.24501170522839272,"score_spread":0.23640096721954124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001032132","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.66425115,0.00037036033,0.2976044,0.0006686651,0.000101509366,0.00006389325,0.00028224595,0.0005455735,0.03611219],"genre_scores_gemma":[0.99373627,0.00007224773,0.0049672946,0.00007216447,0.000026398164,0.000021163814,0.00006959767,0.00005731887,0.0009774199],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996147,0.00007208617,0.000018665118,0.00006981955,0.00015923358,0.00006538786],"domain_scores_gemma":[0.9987919,0.000510448,0.00015002077,0.00029696894,0.00015775178,0.000092976945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008584645,0.00024551738,0.00035303333,0.0007858939,0.0005479053,0.0011979275,0.0009870675,0.00054357667,0.0026822009],"category_scores_gemma":[0.0051698643,0.00025776276,0.0003843892,0.00032189625,0.0015433906,0.0028023978,0.0009238538,0.00081974734,0.0002904592],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008129548,0.00006158238,0.006589716,0.000068480906,0.00002396156,0.00034799057,0.00033087409,0.2749812,0.0065194867,0.7000549,0.001248389,0.00969208],"study_design_scores_gemma":[0.000013285527,0.000023428296,0.003802636,0.000012029356,0.0000045294073,0.00017568961,0.000050861843,0.5932883,0.0019011574,0.3995858,0.0011160693,0.000026216661],"about_ca_topic_score_codex":0.0011008055,"about_ca_topic_score_gemma":0.0007455418,"teacher_disagreement_score":0.0026822009,"about_ca_system_score_codex":0.0008427648,"about_ca_system_score_gemma":0.0005002317,"threshold_uncertainty_score":0.008972883},"labels":[],"label_agreement":null},{"id":"W2001074139","doi":"10.1088/0004-637x/800/2/133","title":"DYNAMICAL PROPERTIES OF COLLISIONLESS STAR STREAMS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics","funders":"","keywords":"Eccentricity (behavior); Angular momentum; Tidal heating; Orbital eccentricity; Scaling; Tidal force; Galaxy; Satellite; Orbit (dynamics)","score_opus":0.01450263624821612,"score_gpt":0.21379878959789822,"score_spread":0.1992961533496821,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001074139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99317294,0.000064784894,0.004965428,0.000035318495,0.0000064274877,0.000021628508,0.00016415396,0.000074509735,0.0014947059],"genre_scores_gemma":[0.9983436,0.00003450018,0.000856092,0.000005124122,0.000009325639,0.000007997581,0.00022349072,0.000020345518,0.000499653],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988616,0.000018546405,0.000012198134,0.000029098563,0.000030849846,0.000023183627],"domain_scores_gemma":[0.9984707,0.0004622981,0.0004125557,0.00010430703,0.00021123333,0.00033889152],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003291715,0.00025841952,0.00026641614,0.0010932351,0.00054403796,0.0013040986,0.00046718237,0.00029669702,0.0012996856],"category_scores_gemma":[0.0042390884,0.000251041,0.00023061795,0.0004615049,0.00064086524,0.00070231734,0.00059162406,0.0002720127,0.0001762386],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007574144,0.00023573246,0.30543813,0.00008989767,0.00013909808,0.0020377534,0.0010699315,0.56696194,0.051052455,0.056474224,0.0012517169,0.014491761],"study_design_scores_gemma":[0.00003671385,0.00009605366,0.043348253,0.000009928497,0.00001535859,0.0002907715,0.00014116685,0.9433563,0.003919531,0.008064991,0.000691532,0.00002947718],"about_ca_topic_score_codex":0.0025828518,"about_ca_topic_score_gemma":0.001173545,"teacher_disagreement_score":0.0025828518,"about_ca_system_score_codex":0.0007776216,"about_ca_system_score_gemma":0.0002604242,"threshold_uncertainty_score":0.0056420565},"labels":[],"label_agreement":null},{"id":"W2001123078","doi":"10.1088/0004-637x/732/1/13","title":"A<i>CHANDRA</i>STUDY OF THE LARGE-SCALE SHOCK AND COOL FILAMENTS IN HYDRA A: EVIDENCE FOR SUBSTANTIAL GAS DREDGE-UP BY THE CENTRAL OUTBURST","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Shock wave; Shock (circulatory); Galaxy cluster; Mach number; Plateau (mathematics); Galaxy; Protein filament; Shock front","score_opus":0.019565289780392684,"score_gpt":0.2354001443451401,"score_spread":0.2158348545647474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001123078","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998934,0.000111312715,0.00013186128,0.000021285836,0.0000031095674,0.000003688328,0.00017313955,0.000025866533,0.00059579505],"genre_scores_gemma":[0.99874145,0.000078122524,0.0005476065,0.000022719043,0.000012312201,0.0000045485344,0.0003309325,0.000011744139,0.0002506768],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999523,0.0000030416054,0.000002764906,0.000013425261,0.000008484367,0.0000199999],"domain_scores_gemma":[0.9996761,0.00004465833,0.00007773369,0.00003670524,0.000035036483,0.00012983673],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010179704,0.00023160117,0.00023995072,0.00069049076,0.00054344424,0.00042738038,0.00031367716,0.00019109811,0.00086942955],"category_scores_gemma":[0.00019484658,0.00013116443,0.00023991322,0.0004270542,0.00027908507,0.00020207645,0.00050711405,0.000370477,0.000170129],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011945765,0.00032839846,0.5742735,0.00015020494,0.00024593645,0.0046246774,0.0008957321,0.0026031244,0.40057284,0.00062856893,0.0013001454,0.013182328],"study_design_scores_gemma":[0.000012315217,0.00016286649,0.9888524,0.000006685649,0.000039447983,0.00074287615,0.00016217011,0.0010873199,0.008011422,0.000095479925,0.00080906745,0.00001797469],"about_ca_topic_score_codex":0.004839426,"about_ca_topic_score_gemma":0.004426846,"teacher_disagreement_score":0.004839426,"about_ca_system_score_codex":0.00021498466,"about_ca_system_score_gemma":0.0001535135,"threshold_uncertainty_score":0.009622514},"labels":[],"label_agreement":null},{"id":"W2001248001","doi":"10.1086/508602","title":"On Universal Halos and the Radial Orbit Instability","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Instability; Orbit (dynamics); Halo; Circular orbit; Universality (dynamical systems); Halo orbit; Radial velocity","score_opus":0.0042035981754539355,"score_gpt":0.18899332393108295,"score_spread":0.18478972575562902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001248001","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.926504,0.0050784643,0.024109622,0.0014777475,0.00006315273,0.000009353672,0.000052202642,0.00017310989,0.042532388],"genre_scores_gemma":[0.9974306,0.0010065442,0.00073115784,0.000067494606,0.000041856467,0.0000042523047,0.0000133478,0.000017151375,0.00068763393],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998534,0.000051564963,0.0000043730383,0.000015075671,0.000033318855,0.00004222979],"domain_scores_gemma":[0.9993111,0.00030429527,0.000118257725,0.00012973697,0.00005924556,0.000077353136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004696182,0.00023446756,0.00027866018,0.0005510642,0.00052758475,0.0006422563,0.00035748878,0.00029033408,0.001439594],"category_scores_gemma":[0.0019133515,0.00011834659,0.00018980789,0.00031218992,0.0023277192,0.0011736886,0.0013338214,0.00044915552,0.0001594924],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013138492,0.000023145212,0.005754257,0.00009120021,0.000034958197,0.00060582254,0.00056393765,0.036701683,0.010392854,0.92506295,0.0015744419,0.019063313],"study_design_scores_gemma":[0.000030435285,0.0000461053,0.0065140575,0.000051331663,0.000018820076,0.00023023473,0.00029894232,0.07871525,0.0032521123,0.9071114,0.003696844,0.00003442254],"about_ca_topic_score_codex":0.0012994101,"about_ca_topic_score_gemma":0.00082603836,"teacher_disagreement_score":0.001439594,"about_ca_system_score_codex":0.00046247197,"about_ca_system_score_gemma":0.0002039105,"threshold_uncertainty_score":0.004815936},"labels":[],"label_agreement":null},{"id":"W2001358528","doi":"10.1086/322324","title":"Cosmic‐Ray Electrons and Positrons from 1 to 100 GeV: Measurements with HEAT and Their Interpretation","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":246,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Cosmic ray; Positron; Antimatter; Electron; Astrophysics; Context (archaeology); Range (aeronautics); Spectral line; Nuclear physics; Astronomy","score_opus":0.009037530989304775,"score_gpt":0.2156220954794959,"score_spread":0.20658456449019114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001358528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99569535,0.00027929246,0.0004250364,0.000057965502,0.0000054705183,0.000003667472,0.00032209585,0.000017586983,0.0031936122],"genre_scores_gemma":[0.9990453,0.00012938977,0.0003651655,0.000009659995,0.0000058233754,0.000002727857,0.00021349864,0.0000048207917,0.00022356954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990547,0.000015231671,0.0000042242,0.000023191484,0.00002606663,0.00002577582],"domain_scores_gemma":[0.999619,0.00010135494,0.00013268738,0.000044367505,0.000060998864,0.00004165569],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016141216,0.0003054689,0.00016195668,0.0012578479,0.00036577074,0.00052110007,0.00028181018,0.00022073723,0.00071243785],"category_scores_gemma":[0.0006526632,0.00021476012,0.00014491791,0.0011877794,0.0005474373,0.00034824086,0.00049659866,0.00032438082,0.00009718674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081041316,0.00005253784,0.9268712,0.0000892023,0.0000945069,0.0005175329,0.0008050107,0.00080215797,0.052976698,0.0034624436,0.0005533823,0.012964942],"study_design_scores_gemma":[0.000012511701,0.00004218988,0.9875327,0.000010434206,0.000030342391,0.00043776858,0.00014700629,0.0006555966,0.008872553,0.0007681037,0.0014797521,0.000011031286],"about_ca_topic_score_codex":0.004902865,"about_ca_topic_score_gemma":0.012155183,"teacher_disagreement_score":0.004902865,"about_ca_system_score_codex":0.00049417274,"about_ca_system_score_gemma":0.00014357563,"threshold_uncertainty_score":0.009748638},"labels":[],"label_agreement":null},{"id":"W2001436498","doi":"10.1088/0004-637x/793/2/95","title":"SUPERNOVA REMNANT W49B AND ITS ENVIRONMENT","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Supernova remnant; Molecular cloud; Supernova; Infrared; Spectral line; Line (geometry); Stars; Astronomy","score_opus":0.007001524633298997,"score_gpt":0.1929105438838562,"score_spread":0.1859090192505572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001436498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988901,0.000097084136,0.000047660575,0.000013015481,0.0000011929053,0.0000014404866,0.00011649396,0.0000045495585,0.0008283758],"genre_scores_gemma":[0.9988663,0.0001026449,0.00009954769,0.000009490136,0.0000060429097,0.000002049415,0.00055195205,0.0000059210183,0.00035605973],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999521,0.000006160228,0.0000026898213,0.000013887717,0.000008999086,0.000016202386],"domain_scores_gemma":[0.99990654,0.0000074284444,0.00003493964,0.000007853322,0.000009449888,0.000033776992],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010339384,0.00015803336,0.00023540633,0.00045205097,0.00027490247,0.0005734709,0.00017969734,0.00021251418,0.0009919552],"category_scores_gemma":[0.0002121415,0.00007363044,0.00018112287,0.0004523866,0.00019650579,0.00026360803,0.0005169649,0.00019399644,0.00028883712],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039335497,0.00012982498,0.95083505,0.000038846036,0.00010915929,0.0025290598,0.00040427787,0.0018431421,0.030465089,0.0012352546,0.0005729242,0.011444014],"study_design_scores_gemma":[0.000013934943,0.0001293028,0.99190146,0.0000082591105,0.000028658274,0.0008354745,0.00042209387,0.0024236212,0.00089053524,0.0002987138,0.0030357982,0.000011988158],"about_ca_topic_score_codex":0.006884531,"about_ca_topic_score_gemma":0.0074555604,"teacher_disagreement_score":0.006884531,"about_ca_system_score_codex":0.00021726356,"about_ca_system_score_gemma":0.00011556286,"threshold_uncertainty_score":0.013688922},"labels":[],"label_agreement":null},{"id":"W2001452877","doi":"10.1086/321704","title":"Evolution of Carbon Dust in Aromatic Infrared Emission Sources: Formation of Nanodiamonds","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Infrared; Cosmic dust; Astrophysics; Astrobiology; Astrochemistry; Carbon fibers; Astronomy; Circumstellar dust; Carbon star; Interstellar medium; Stars; Galaxy; Composite number","score_opus":0.008735891211586806,"score_gpt":0.22055165403176574,"score_spread":0.21181576282017894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001452877","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987697,0.000058547164,0.00038891454,0.000010559742,0.0000016040568,0.000007171847,0.00011432028,0.000022784823,0.0006264372],"genre_scores_gemma":[0.99870574,0.000024208099,0.0006416236,0.000008500864,0.0000017460924,0.000005895693,0.00020630918,0.000009396999,0.00039656076],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993503,0.0000030600572,0.0000024036995,0.000023493316,0.000019066898,0.000016903648],"domain_scores_gemma":[0.9998417,0.00002331854,0.00003493251,0.000011825536,0.00004009396,0.00004816114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000076608085,0.00016250397,0.00013471681,0.00038644118,0.00026496037,0.0003317524,0.00029068885,0.00031653952,0.0005606159],"category_scores_gemma":[0.00016091764,0.00014489071,0.00013565434,0.00014340926,0.00020165686,0.00014098389,0.00016101217,0.00023840347,0.00017376387],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010233591,0.00002768272,0.0137210395,0.00001480382,0.000007108636,0.00013024012,0.000055443186,0.00014529185,0.98466194,0.00010579676,0.000037864214,0.0009904217],"study_design_scores_gemma":[0.000029575733,0.00017214862,0.31887358,0.000006820535,0.000018417097,0.000510241,0.00018817371,0.00281861,0.6759941,0.00021694963,0.0011591444,0.000012264301],"about_ca_topic_score_codex":0.0013791878,"about_ca_topic_score_gemma":0.0013741127,"teacher_disagreement_score":0.0013791878,"about_ca_system_score_codex":0.00047324196,"about_ca_system_score_gemma":0.00011485799,"threshold_uncertainty_score":0.0034336448},"labels":[],"label_agreement":null},{"id":"W2001484894","doi":"10.1086/422499","title":"Synchrotron versus Compton Interpretations for Extended X‐Ray Jets","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Blazar; Quasar; Synchrotron; Astrophysical jet; Electron; Synchrotron radiation; Collimated light; Neutrino; Lorentz factor; Cosmic microwave background","score_opus":0.012488936656460189,"score_gpt":0.26072811229281423,"score_spread":0.24823917563635403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001484894","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2911328,0.027070966,0.18053052,0.04284489,0.0035683394,0.00012791254,0.0006249561,0.001021899,0.45307767],"genre_scores_gemma":[0.952783,0.0046764454,0.010931338,0.0026414057,0.0029962964,0.000077694254,0.00022306902,0.00015182869,0.02551901],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99956506,0.000099867204,0.00002751602,0.00008557448,0.00012687726,0.0000950479],"domain_scores_gemma":[0.9984049,0.00076035404,0.00024253567,0.00026571593,0.00017207277,0.00015436455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010963252,0.00058879756,0.0004154922,0.0011594583,0.000839884,0.004678897,0.001836748,0.0024669243,0.014622663],"category_scores_gemma":[0.0021951287,0.000276298,0.00075990445,0.00095881236,0.006589781,0.0048543112,0.0026304128,0.0016561428,0.0011643254],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027302807,0.00001373834,0.00092144654,0.000051351242,0.000004641466,0.0004375677,0.00049796095,0.00044932863,0.00048101915,0.9924689,0.0009912367,0.0036556108],"study_design_scores_gemma":[0.00004701243,0.000027823542,0.0020787423,0.000052765976,0.000009839577,0.0010622342,0.00042897047,0.0032273706,0.00020565953,0.97218806,0.020653235,0.000018303052],"about_ca_topic_score_codex":0.00065859826,"about_ca_topic_score_gemma":0.00059619726,"teacher_disagreement_score":0.014622663,"about_ca_system_score_codex":0.0007857292,"about_ca_system_score_gemma":0.00044933363,"threshold_uncertainty_score":0.04891765},"labels":[],"label_agreement":null},{"id":"W2001506720","doi":"10.1086/321686","title":"High‐Latitude H<scp>i</scp>in NGC 2613: Structure and Dynamics","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Barred spiral galaxy; Interacting galaxy; Spiral galaxy; Galaxy formation and evolution","score_opus":0.0038084383916644044,"score_gpt":0.19431885229191248,"score_spread":0.1905104139002481,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001506720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990933,0.00003806964,0.0000959207,0.000008946718,6.651492e-7,0.0000015949665,0.00011476604,0.000009166755,0.0006375085],"genre_scores_gemma":[0.9990564,0.000036700545,0.00024394722,0.0000045836955,0.00000200397,0.0000016312682,0.0003761409,0.0000036999343,0.00027485224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995697,0.0000022711565,0.0000015229425,0.000012654477,0.0000074032587,0.000019163552],"domain_scores_gemma":[0.9997278,0.000011723515,0.00012038425,0.000017230497,0.000036742797,0.00008612439],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000046820976,0.00011980061,0.00009744416,0.00041301065,0.00036184024,0.00039875248,0.00014036777,0.00013625131,0.0008333474],"category_scores_gemma":[0.00021617192,0.00011779715,0.00008560334,0.00077327364,0.0003321451,0.00014593171,0.00028717288,0.00014213636,0.0002856263],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001388472,0.000041545736,0.93917114,0.000022052654,0.000021760032,0.00044284292,0.000575281,0.0006279174,0.046542488,0.0004140889,0.00053842244,0.011463589],"study_design_scores_gemma":[0.0000020403224,0.000015857462,0.99778324,0.0000027927395,0.000003921181,0.00021983794,0.00008336511,0.000329672,0.0009722223,0.000057392306,0.0005273819,0.0000022561835],"about_ca_topic_score_codex":0.01886344,"about_ca_topic_score_gemma":0.030054465,"teacher_disagreement_score":0.01886344,"about_ca_system_score_codex":0.0005002901,"about_ca_system_score_gemma":0.00021726087,"threshold_uncertainty_score":0.037507296},"labels":[],"label_agreement":null},{"id":"W2001528761","doi":"10.1086/342825","title":"A Universal Temperature Profile for Galaxy Clusters","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Radiative cooling; Astrophysics; Cluster (spacecraft); Galaxy cluster; Supernova; Gaussian; Polytropic process; Galaxy; Isothermal process; Statistical physics; Thermodynamics; Quantum mechanics","score_opus":0.007377983498217791,"score_gpt":0.19719078927782394,"score_spread":0.18981280577960613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001528761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9731409,0.0001482127,0.021314051,0.00013894576,0.000006170584,0.000021667904,0.00029626302,0.00027328896,0.004660474],"genre_scores_gemma":[0.99715364,0.00003304226,0.0022612072,0.000011175883,0.0000018574407,0.000008658179,0.00016982692,0.000029488087,0.00033109495],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99989283,0.00001456292,0.0000025939469,0.000035221452,0.000022419226,0.000032366734],"domain_scores_gemma":[0.99970955,0.000054546217,0.00006231008,0.000074964875,0.00005777206,0.00004076706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025377673,0.00020483613,0.00017076268,0.00031525202,0.00030944357,0.0005411405,0.00059771666,0.00032645444,0.0011448201],"category_scores_gemma":[0.0016708035,0.00012559617,0.00033649278,0.0003083804,0.0005625962,0.00048397935,0.00040064106,0.00034000314,0.00021513106],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024401954,0.00006149786,0.18156531,0.00007330803,0.000054442586,0.00029618543,0.000987409,0.68992686,0.038705047,0.0686128,0.0016849516,0.017788252],"study_design_scores_gemma":[0.000024787714,0.00008683339,0.085724965,0.000021532818,0.000012861572,0.0002245248,0.00018384574,0.89162844,0.0063037947,0.013441287,0.0023097992,0.000037312435],"about_ca_topic_score_codex":0.008449357,"about_ca_topic_score_gemma":0.0046379105,"teacher_disagreement_score":0.008449357,"about_ca_system_score_codex":0.0008291838,"about_ca_system_score_gemma":0.00032136793,"threshold_uncertainty_score":0.016800344},"labels":[],"label_agreement":null},{"id":"W2001611906","doi":"10.1088/0004-637x/792/1/59","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. V. MODELING THE DYNAMICS OF M87 WITH THE MADE-TO-MEASURE METHOD","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Velocity dispersion; Dark matter; Galaxy; RADIUS; Virgo Cluster; Elliptical galaxy; Star cluster; Galaxy cluster","score_opus":0.02210061912352481,"score_gpt":0.2360035410714643,"score_spread":0.21390292194793947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001611906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7622858,0.0019529918,0.083650954,0.0036027506,0.00034140117,0.0004765408,0.09635333,0.005021937,0.046314236],"genre_scores_gemma":[0.92871726,0.00030529298,0.03294752,0.00029412346,0.000091688846,0.00028449926,0.024693558,0.00066994457,0.011996185],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999819,0.000073449446,0.0000050020935,0.000037363985,0.000028981345,0.000036286052],"domain_scores_gemma":[0.99970835,0.00006980112,0.000051168754,0.00006155923,0.00005247053,0.000056742716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00082210114,0.00034979056,0.00042125894,0.00085472217,0.0004559083,0.0007823559,0.0015138087,0.0007687946,0.0028157737],"category_scores_gemma":[0.001899794,0.0002765286,0.0007017633,0.0012662098,0.00019889543,0.00058994605,0.00073820306,0.0005883146,0.0011671865],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012939662,0.00010798426,0.11061104,0.00010884926,0.00023666212,0.000091153444,0.00022977116,0.78747994,0.00041455997,0.024013916,0.047775686,0.028801065],"study_design_scores_gemma":[0.0000509949,0.000024955769,0.05379569,0.000043164633,0.000035250476,0.0000398627,0.00016950366,0.91042906,0.0002290569,0.011753191,0.023392716,0.00003653513],"about_ca_topic_score_codex":0.2105381,"about_ca_topic_score_gemma":0.12721203,"teacher_disagreement_score":0.2105381,"about_ca_system_score_codex":0.0014409944,"about_ca_system_score_gemma":0.0011439774,"threshold_uncertainty_score":0.41862524},"labels":[],"label_agreement":null},{"id":"W2001636212","doi":"10.1088/0004-637x/770/1/13","title":"REDSHIFT 6.4 HOST GALAXIES OF 10<sup>8</sup>SOLAR MASS BLACK HOLES: LOW STAR FORMATION RATE AND DYNAMICAL MASS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Redshift; Galaxy; Star formation; Black hole (networking); Eddington luminosity; Luminosity; Stellar mass; Intermediate-mass black hole","score_opus":0.00757573428082129,"score_gpt":0.202962981256627,"score_spread":0.19538724697580573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001636212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939421,0.00013324802,0.00037162774,0.00010696593,0.00002391889,0.000011342705,0.0013824702,0.00029171788,0.0037366499],"genre_scores_gemma":[0.9951166,0.0000439597,0.00027347842,0.000034708122,0.000030815103,0.000003125507,0.0015661255,0.000021049815,0.0029101095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999263,0.000005111769,0.0000029621237,0.000016175909,0.00001377704,0.000035606707],"domain_scores_gemma":[0.9994973,0.000053278858,0.00017163465,0.000034984343,0.000043425633,0.00019949215],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001306428,0.00027363712,0.00024380985,0.0010759014,0.0003345247,0.0005521739,0.00026646059,0.00030322306,0.009908603],"category_scores_gemma":[0.000379735,0.00012944247,0.00017609347,0.00060803565,0.00021174843,0.00023723594,0.00031350646,0.00020693919,0.0023292967],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050882617,0.00011367959,0.9544333,0.000049783997,0.000055375167,0.00043446815,0.00035247594,0.00015068876,0.027154805,0.0009041787,0.002600848,0.013241511],"study_design_scores_gemma":[0.000014182901,0.000047455353,0.9945539,0.0000020856412,0.000021046782,0.00038910288,0.00021986746,0.00034256832,0.0026073167,0.00020226378,0.0015970464,0.0000031694233],"about_ca_topic_score_codex":0.0020857658,"about_ca_topic_score_gemma":0.0034621153,"teacher_disagreement_score":0.009908603,"about_ca_system_score_codex":0.00016313414,"about_ca_system_score_gemma":0.00007778309,"threshold_uncertainty_score":0.033147633},"labels":[],"label_agreement":null},{"id":"W2001717952","doi":"10.1086/499931","title":"Dry Mergers in GEMS: The Dynamical Evolution of Massive Early‐Type Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":313,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy merger; Galaxy; Astronomy; Galaxy formation and evolution; Elliptical galaxy; Luminosity; Hubble space telescope; Redshift","score_opus":0.00416249832613734,"score_gpt":0.1961721491178953,"score_spread":0.19200965079175797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001717952","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997738,0.000016896749,0.000063492655,0.000004092712,2.719617e-7,0.0000011446708,0.00006120505,0.000005410929,0.00007381091],"genre_scores_gemma":[0.99924767,0.000015036853,0.00029276227,0.0000034182979,0.000001150943,0.0000017499312,0.0003627004,0.000002980469,0.000072393705],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987376,0.0000244078,0.000008698471,0.00004256662,0.000023056735,0.00002757412],"domain_scores_gemma":[0.9994578,0.00008351928,0.00018561626,0.00006375146,0.00004330213,0.00016604326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004423146,0.00020549068,0.00024219912,0.0006818895,0.00032727496,0.0004956899,0.00033024087,0.00019150178,0.0002949051],"category_scores_gemma":[0.00088575087,0.0002077622,0.0002476403,0.00060572487,0.0002746832,0.00036144254,0.0006439814,0.00021366662,0.00009336077],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016798385,0.000049551294,0.9744086,0.000010405838,0.00006245867,0.00013184549,0.00046002233,0.005534955,0.015356603,0.00032955373,0.0000770597,0.0034109592],"study_design_scores_gemma":[0.000010544723,0.000080019796,0.98505026,0.0000024353892,0.000016235146,0.00013165557,0.0001305801,0.012176228,0.0017762509,0.00017162973,0.00044450886,0.000009816903],"about_ca_topic_score_codex":0.007871924,"about_ca_topic_score_gemma":0.0108455885,"teacher_disagreement_score":0.007871924,"about_ca_system_score_codex":0.0005911362,"about_ca_system_score_gemma":0.0002092872,"threshold_uncertainty_score":0.01565224},"labels":[],"label_agreement":null},{"id":"W2001872772","doi":"10.1086/323369","title":"<i>HST</i>STIS Observations of PG 0946+301: The Highest Quality UV Spectrum of a BALQSO","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Space Telescope Imaging Spectrograph; Metallicity; Astrophysics; Physics; Spectrograph; Hubble space telescope; Spectral line; Astronomy; Ionization; Stars; Ion","score_opus":0.03162140360869516,"score_gpt":0.2585448808504617,"score_spread":0.2269234772417665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001872772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.939992,0.0005139511,0.0022284994,0.00041389867,0.00005822821,0.000047674825,0.034398478,0.00067924015,0.02166805],"genre_scores_gemma":[0.9543901,0.00038030354,0.0073813745,0.0001694767,0.00016380972,0.000020675454,0.034122597,0.00009182717,0.0032798352],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999616,0.0000026452014,0.0000035005148,0.0000068893905,0.000013761164,0.000011625663],"domain_scores_gemma":[0.99981326,0.000011370384,0.000058591515,0.00002550113,0.00002450687,0.00006669159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010907962,0.00018804792,0.00015089597,0.0010706756,0.000339951,0.0003725473,0.00016256038,0.00017071806,0.0053706802],"category_scores_gemma":[0.0001919405,0.00008103538,0.00010416972,0.0009601146,0.00018673179,0.00023761035,0.00032924968,0.00023693801,0.0013753937],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060156063,0.0002887455,0.68857193,0.00029246224,0.00010573845,0.0020442288,0.00089068385,0.0027046464,0.13331692,0.0016734673,0.045739256,0.12377034],"study_design_scores_gemma":[0.000017921855,0.00010583343,0.9686775,0.000013798958,0.000023462524,0.0010606012,0.00012372722,0.0008677158,0.0061710086,0.0003433904,0.02258153,0.000013562604],"about_ca_topic_score_codex":0.0036098268,"about_ca_topic_score_gemma":0.012058817,"teacher_disagreement_score":0.0053706802,"about_ca_system_score_codex":0.00018563807,"about_ca_system_score_gemma":0.00010721432,"threshold_uncertainty_score":0.017966688},"labels":[],"label_agreement":null},{"id":"W2001915955","doi":"10.1086/590365","title":"Simultaneous Determination of the Cosmic Ray Ionization Rate and Fractional Ionization in DR 21(OH)","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Western University","funders":"","keywords":"Ionization; Cosmic ray; Abundance (ecology); Chemistry; Atomic physics; Natural abundance; Astrophysics; Physics; Mass spectrometry; Ion","score_opus":0.008028215673981575,"score_gpt":0.22646102243336058,"score_spread":0.218432806759379,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001915955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94922554,0.00050066167,0.04557452,0.00001839308,0.000009273917,0.000033051485,0.00039913147,0.00030172247,0.0039375904],"genre_scores_gemma":[0.97735745,0.00024425137,0.021265173,0.000010812432,0.0000077851855,0.000023034274,0.00036399908,0.000036054196,0.0006915368],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998398,0.000013020402,0.0000069973303,0.000052630694,0.00007317466,0.00001435299],"domain_scores_gemma":[0.9996867,0.000042967946,0.00010924053,0.00008370005,0.000044236738,0.000033154007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021389817,0.0003526315,0.00017788772,0.00093665806,0.0001452465,0.00025886067,0.0004890584,0.00015566588,0.0005570817],"category_scores_gemma":[0.0005196978,0.00017534972,0.00018942406,0.000374444,0.00013525343,0.0002718294,0.00050860137,0.00019559822,0.00022668063],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020160619,0.00006048165,0.32507864,0.00009991186,0.00017788909,0.00035029894,0.00024470076,0.017554672,0.53546494,0.0025251028,0.0002246776,0.11801711],"study_design_scores_gemma":[0.00003971589,0.0002515034,0.4870579,0.000024325558,0.00010890393,0.0010732883,0.00012923192,0.17309116,0.32899985,0.0019994979,0.007091017,0.00013355321],"about_ca_topic_score_codex":0.0022434006,"about_ca_topic_score_gemma":0.0046392535,"teacher_disagreement_score":0.0022434006,"about_ca_system_score_codex":0.00027655548,"about_ca_system_score_gemma":0.0001627915,"threshold_uncertainty_score":0.0044606924},"labels":[],"label_agreement":null},{"id":"W2001958185","doi":"10.1086/528681","title":"Where Centaurus A Gets Its X-Ray Knottiness","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"History and Developments in Astronomy","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Centaurus A; Red shift; Luminosity; Astrometry; X-ray astronomy","score_opus":0.011441691926961194,"score_gpt":0.22163364145826422,"score_spread":0.21019194953130302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2001958185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5783331,0.005617913,0.0028868252,0.010167402,0.0024219453,0.00002473017,0.00053372537,0.0010351441,0.3989793],"genre_scores_gemma":[0.97692966,0.00050282653,0.00039359878,0.0005713281,0.0002836426,0.000005615973,0.00011700457,0.000116262556,0.021080025],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99950016,0.00006702343,0.000016694401,0.0001141615,0.000110247805,0.00019169463],"domain_scores_gemma":[0.9987203,0.00015846468,0.00020704561,0.00023194158,0.00023927087,0.00044295055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000612496,0.0002443679,0.0002891876,0.001502375,0.0023731038,0.006508767,0.0004158696,0.0011785816,0.030494742],"category_scores_gemma":[0.004052665,0.00021532767,0.00026087178,0.0006809725,0.0029707174,0.004564209,0.0031372788,0.0015708384,0.0055724955],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011459079,0.00012487615,0.092317946,0.00043574508,0.000105607505,0.003534957,0.015808417,0.001593871,0.031138215,0.64465046,0.05829282,0.1508512],"study_design_scores_gemma":[0.0000763411,0.00033157744,0.310756,0.00067080144,0.00008551265,0.0057227123,0.017006146,0.0012288765,0.013583772,0.32772496,0.32253906,0.000274273],"about_ca_topic_score_codex":0.0039914157,"about_ca_topic_score_gemma":0.002462918,"teacher_disagreement_score":0.030494742,"about_ca_system_score_codex":0.0013427256,"about_ca_system_score_gemma":0.00048887753,"threshold_uncertainty_score":0.10201508},"labels":[],"label_agreement":null},{"id":"W2002191346","doi":"10.1088/0004-637x/728/2/83","title":"LOW-MULTIPLICITY BURST SEARCH AT THE SUDBURY NEUTRINO OBSERVATORY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; University of Guelph; Laurentian University; University of Alberta; Snolab; Queen's University; TRIUMF; Carleton University","funders":"Science and Technology Facilities Council; Canada Research Chairs; Industry Canada; Alfred P. Sloan Foundation; Strong; U.S. Department of Energy","keywords":"Observatory; Physics; Supernova; Multiplicity (mathematics); Neutrino; Neutrino detector; Astrophysics; Astronomy; Detector; Nuclear physics; Neutrino oscillation; Optics","score_opus":0.04805516535786091,"score_gpt":0.2841248590300898,"score_spread":0.2360696936722289,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002191346","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98934233,0.00034790934,0.002772408,0.00009711072,0.000016345963,0.000064867054,0.00404379,0.00011574228,0.0031994993],"genre_scores_gemma":[0.9800903,0.00014806444,0.009356773,0.00005839273,0.000026691037,0.00003762518,0.008258855,0.00003639843,0.0019869148],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991756,0.00014297289,0.000047922673,0.00020955053,0.000261363,0.00016265646],"domain_scores_gemma":[0.997658,0.000437128,0.00051609543,0.00028406942,0.0005231398,0.0005815567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012232215,0.000388712,0.0005801617,0.0016292932,0.0014109939,0.000983328,0.00067374605,0.000365409,0.0023159657],"category_scores_gemma":[0.0021416142,0.00032679542,0.0003312685,0.0014544824,0.00027824444,0.0005278707,0.0011569908,0.00050877786,0.0005017873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002266712,0.00023218157,0.87546456,0.00009807616,0.00026356432,0.0015850194,0.00037257498,0.001172863,0.07331904,0.000948055,0.0037346988,0.04054264],"study_design_scores_gemma":[0.0002820941,0.00086179026,0.91291225,0.000026926347,0.00019251405,0.0022119216,0.00032026216,0.0087178955,0.05532086,0.0009373903,0.018101553,0.0001145684],"about_ca_topic_score_codex":0.025879174,"about_ca_topic_score_gemma":0.06483049,"teacher_disagreement_score":0.97412086,"about_ca_system_score_codex":0.00092361786,"about_ca_system_score_gemma":0.0010973389,"threshold_uncertainty_score":0.051457107},"labels":[],"label_agreement":null},{"id":"W2002253735","doi":"10.1086/508140","title":"The First DIRECT Distance Determination to a Detached Eclipsing Binary in M33","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Distance modulus; Photometry (optics); Binary number; Spectroscopy; Stars; Apparent magnitude; Light curve; Binary star; Main sequence","score_opus":0.007482524604273838,"score_gpt":0.22384943728325418,"score_spread":0.21636691267898034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002253735","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9758656,0.0007366651,0.00051514397,0.0016126669,0.00062958733,0.000042938464,0.00065376196,0.000043332064,0.019900227],"genre_scores_gemma":[0.98832583,0.00011124248,0.00051409384,0.0004156053,0.00018477811,0.0000070342817,0.0007486887,0.000019822313,0.009672936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979514,0.000015863136,0.000015344669,0.000059325324,0.000049645372,0.00006461092],"domain_scores_gemma":[0.9991529,0.000100429424,0.00011401544,0.00009613377,0.00026771319,0.00026880077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019465995,0.00020034023,0.0003469852,0.00057562935,0.0017575703,0.0006975862,0.000527221,0.0017823398,0.009523056],"category_scores_gemma":[0.0013195832,0.00017217612,0.00019731236,0.00045867436,0.00041680032,0.00048270222,0.0010353808,0.0009407314,0.0036640235],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031593991,0.00058734504,0.58017224,0.0007523808,0.000107582215,0.057203814,0.007245018,0.00038557764,0.1484022,0.0058720843,0.0403355,0.15577683],"study_design_scores_gemma":[0.00010418019,0.0014354171,0.88325405,0.000092736154,0.000058591184,0.01823443,0.0021940863,0.00037139346,0.013744488,0.0011439703,0.079311855,0.00005473359],"about_ca_topic_score_codex":0.0037685563,"about_ca_topic_score_gemma":0.0069263643,"teacher_disagreement_score":0.009523056,"about_ca_system_score_codex":0.00041965232,"about_ca_system_score_gemma":0.0003579386,"threshold_uncertainty_score":0.03185785},"labels":[],"label_agreement":null},{"id":"W2002265177","doi":"10.1086/324036","title":"GSH 138−01−94: An Old Supernova Remnant in the Far Outer Galaxy","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Queen's University","funders":"","keywords":"Supernova remnant; Interstellar medium; Supernova; Galaxy; Surface brightness; Galactic plane; Stars; RADIUS","score_opus":0.01219313025056292,"score_gpt":0.22726536298026895,"score_spread":0.21507223272970602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002265177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99758804,0.00007420538,0.000047676815,0.00004127895,0.0000058897517,0.000011798386,0.00036707064,0.000018196242,0.0018457876],"genre_scores_gemma":[0.99737996,0.000088244204,0.00016102428,0.000039171202,0.000008895501,0.0000043854916,0.0011357149,0.000010090205,0.0011725195],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990296,0.000003900222,0.0000061137252,0.000020954943,0.000028167908,0.00003791155],"domain_scores_gemma":[0.999689,0.000007508413,0.00005744081,0.000024028204,0.000023046032,0.00019905259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013756921,0.00037736513,0.00043147683,0.0007428812,0.0010736397,0.000676367,0.0005493043,0.0002942656,0.0019642855],"category_scores_gemma":[0.00024850242,0.00018279035,0.00025930852,0.00084368396,0.0004898609,0.00018574731,0.000801716,0.00040212128,0.0007200591],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007318078,0.00034310133,0.9487112,0.000054318964,0.00010550864,0.012085307,0.0015104222,0.00027938973,0.016951414,0.00089799374,0.0016386786,0.016690867],"study_design_scores_gemma":[0.000030183088,0.00029459936,0.985107,0.000012030793,0.000030465599,0.0060204966,0.00074043695,0.00013555842,0.0008462546,0.00013251333,0.0066357753,0.000014685013],"about_ca_topic_score_codex":0.10321726,"about_ca_topic_score_gemma":0.093371354,"teacher_disagreement_score":0.10321726,"about_ca_system_score_codex":0.0012213918,"about_ca_system_score_gemma":0.000551916,"threshold_uncertainty_score":0.20523292},"labels":[],"label_agreement":null},{"id":"W2002295772","doi":"10.1088/0004-637x/716/1/97","title":"<i>SWIFT</i>-BAT OBSERVATIONS OF THE RECENTLY DISCOVERED MAGNETAR SGR 0501+4516","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Magnetar; Astrophysics; Black-body radiation; RADIUS; Photon; Photosphere; Neutron star; Gamma-ray burst; Spectral line; Photon energy; Radiation; Astronomy; Optics","score_opus":0.014177155003344518,"score_gpt":0.285235057818162,"score_spread":0.27105790281481745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002295772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99718946,0.00017600103,0.0003737246,0.000040449246,0.000011758542,0.000007796115,0.00100899,0.00006993283,0.0011217936],"genre_scores_gemma":[0.9943619,0.00010470859,0.0018153318,0.000041854426,0.000026414129,0.000013642705,0.0030995668,0.00002347167,0.00051305746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998336,0.000020220172,0.000016935754,0.00004736627,0.000049216313,0.00003269281],"domain_scores_gemma":[0.9994936,0.000031963402,0.00025717716,0.000055189266,0.000057934354,0.00010418829],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000339908,0.0004928755,0.00033662803,0.0010530169,0.00037947265,0.00068602693,0.00055528595,0.00039261888,0.0009171151],"category_scores_gemma":[0.00049979246,0.00024657138,0.0004691945,0.00056909205,0.00021814469,0.00026195595,0.0004911829,0.0002920949,0.00049240055],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042660406,0.00016266743,0.91411054,0.00010077563,0.00026568724,0.00075157144,0.00026832678,0.0033605334,0.06504235,0.00028230116,0.0018913676,0.013337368],"study_design_scores_gemma":[0.000027900607,0.00018184946,0.9864411,0.000017257855,0.00008556504,0.0008458032,0.000111265865,0.0050467732,0.0042082504,0.000114697476,0.0028928742,0.00002672452],"about_ca_topic_score_codex":0.0059703407,"about_ca_topic_score_gemma":0.018223869,"teacher_disagreement_score":0.0059703407,"about_ca_system_score_codex":0.0005843162,"about_ca_system_score_gemma":0.00018950245,"threshold_uncertainty_score":0.011871159},"labels":[],"label_agreement":null},{"id":"W2002298511","doi":"10.1086/497119","title":"Gemini Spectroscopy of Supernovae from the Supernova Legacy Survey: Improving High‐Redshift Supernova Selection and Classification","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":226,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"Physics; Redshift; Supernova; Galaxy; Astrophysics; Dark energy; Astronomy; Cosmology","score_opus":0.015762692303623246,"score_gpt":0.2405821864858742,"score_spread":0.22481949418225095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002298511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97462386,0.0011894892,0.008589278,0.000529355,0.00010780315,0.00009169776,0.009067384,0.001294895,0.004506174],"genre_scores_gemma":[0.92799264,0.0015116973,0.04427025,0.0002836409,0.00031092376,0.00009597392,0.020684734,0.00030903096,0.004541077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996049,0.00008961893,0.000044269244,0.00009408399,0.00008381117,0.00008339664],"domain_scores_gemma":[0.9979254,0.00030102074,0.00048520725,0.00053869386,0.00043232585,0.00031733813],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027790307,0.00051073334,0.0004943932,0.0031208494,0.0004427867,0.0011045533,0.0005426089,0.00047518278,0.0027258433],"category_scores_gemma":[0.0023785876,0.00041224758,0.00039278172,0.0017361523,0.000094954004,0.0006704058,0.000982577,0.00032256288,0.0008877068],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085290073,0.00012216278,0.84705126,0.00013395784,0.00019957148,0.00013730377,0.0002433323,0.00051550067,0.04447525,0.00046479664,0.008509343,0.09729457],"study_design_scores_gemma":[0.000042220257,0.000063265616,0.98049885,0.000015605981,0.00018502443,0.0003874942,0.00010076166,0.00280508,0.008621586,0.0003558886,0.006897887,0.00002619084],"about_ca_topic_score_codex":0.0032303804,"about_ca_topic_score_gemma":0.013851912,"teacher_disagreement_score":0.0032303804,"about_ca_system_score_codex":0.00025595663,"about_ca_system_score_gemma":0.00031557947,"threshold_uncertainty_score":0.0146971345},"labels":[],"label_agreement":null},{"id":"W2002504587","doi":"10.1088/0004-637x/721/1/90","title":"SPT-CL J0546-5345: A MASSIVE<i>z</i>&gt;1 GALAXY CLUSTER SELECTED VIA THE SUNYAEV-ZEL'DOVICH EFFECT WITH THE SOUTH POLE TELESCOPE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; South Pole Telescope; Astrophysics; Galaxy cluster; Cluster (spacecraft); Velocity dispersion; Redshift; Telescope; Galaxy; Sunyaev–Zel'dovich effect; Brightest cluster galaxy; Astronomy","score_opus":0.0026546685149219634,"score_gpt":0.18482561599627684,"score_spread":0.18217094748135487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002504587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99667597,0.00005809019,0.00019806545,0.000072499126,0.000022858116,0.000013916446,0.0012469889,0.00005517894,0.0016565007],"genre_scores_gemma":[0.9952304,0.00004352643,0.0005536491,0.00005867374,0.00003488476,0.0000058782593,0.0033008626,0.000018898212,0.00075326406],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997384,0.000010711942,0.00001016968,0.00008033842,0.000084409075,0.00007599915],"domain_scores_gemma":[0.9992873,0.000019763886,0.00023075021,0.000056425164,0.000048616723,0.00035724044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018181327,0.00028219545,0.00037428024,0.0010855193,0.0011113802,0.0006819489,0.0005860916,0.000311244,0.0027654937],"category_scores_gemma":[0.00034478842,0.0001675797,0.00020883807,0.0009128307,0.00042257534,0.00029168164,0.001079158,0.00037882096,0.0010840079],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039236827,0.00020505024,0.94152325,0.000053533062,0.0000881715,0.0032539673,0.00076163944,0.00045349286,0.028719611,0.0009622646,0.011669608,0.011916976],"study_design_scores_gemma":[0.000039007064,0.00013820516,0.9859678,0.0000068438076,0.000023420927,0.0022916773,0.00028710387,0.0016580754,0.0028329205,0.00016242871,0.00657583,0.000016680526],"about_ca_topic_score_codex":0.013105492,"about_ca_topic_score_gemma":0.02007365,"teacher_disagreement_score":0.013105492,"about_ca_system_score_codex":0.0005511399,"about_ca_system_score_gemma":0.0002801637,"threshold_uncertainty_score":0.026058376},"labels":[],"label_agreement":null},{"id":"W2002609659","doi":"10.1086/497286","title":"Intermediate‐Mass Black Hole(s) and Stellar Orbits in the Galactic Center","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galactic Center; Supermassive black hole; Stars; Black hole (networking); Eccentricity (behavior); Orbital eccentricity; Astronomy; Stellar dynamics; Orbit (dynamics); Galactic plane; Galaxy","score_opus":0.011604417764123336,"score_gpt":0.23251493996802514,"score_spread":0.2209105222039018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002609659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938159,0.00019941066,0.0024332274,0.00011237375,0.000016552478,0.000006872739,0.00007218863,0.000068725334,0.003274657],"genre_scores_gemma":[0.9978759,0.000077533565,0.0016447979,0.000023595852,0.000005079858,0.000003474949,0.000058867987,0.000021157157,0.0002895476],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999343,0.000013610981,0.0000030337985,0.000014458585,0.0000141407145,0.000020401756],"domain_scores_gemma":[0.9997464,0.000084799874,0.000052091895,0.000025812207,0.000037766724,0.00005310255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029418874,0.00029995045,0.00047509492,0.0003161013,0.00049612246,0.0006807061,0.0006947963,0.00062306103,0.0012104997],"category_scores_gemma":[0.0013451184,0.00021770979,0.00039003938,0.00029640607,0.0006573084,0.0005753414,0.00055562373,0.00042221477,0.000111346235],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046729652,0.00015662269,0.062497757,0.000081791535,0.00013097176,0.00048068713,0.0003448784,0.89935195,0.0057111518,0.022045525,0.001009787,0.007721585],"study_design_scores_gemma":[0.00016080291,0.00012710129,0.017701322,0.000021484515,0.000038898128,0.00006014143,0.0001518209,0.9757229,0.0014885347,0.0035831714,0.0009235068,0.00002033568],"about_ca_topic_score_codex":0.041191835,"about_ca_topic_score_gemma":0.015749479,"teacher_disagreement_score":0.041191835,"about_ca_system_score_codex":0.00060635305,"about_ca_system_score_gemma":0.0006391116,"threshold_uncertainty_score":0.08190417},"labels":[],"label_agreement":null},{"id":"W2002627459","doi":"10.1086/381722","title":"Investigating the Origins of Dark Matter Halo Density Profiles","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Halo; Physics; Angular momentum; Dark matter; Cold dark matter; Accretion (finance); Astrophysics; Classical mechanics; Galaxy","score_opus":0.008633883341417485,"score_gpt":0.21268582313833256,"score_spread":0.20405193979691508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002627459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98526263,0.00012868027,0.011231225,0.0001421873,0.000004514748,0.000013495541,0.00009450909,0.00014612774,0.002976738],"genre_scores_gemma":[0.99842644,0.00004265692,0.0012665789,0.000008937821,0.0000015549418,0.0000035113644,0.000043662665,0.000018435943,0.00018833467],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999058,0.000023703136,0.0000037372774,0.00001644617,0.00002332555,0.000026977466],"domain_scores_gemma":[0.9992649,0.00025491774,0.00016050282,0.000087481596,0.00011771397,0.00011454911],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055033225,0.0002769938,0.0002243757,0.0006397354,0.00030008546,0.00077442697,0.00045181057,0.00036098505,0.00058393704],"category_scores_gemma":[0.0038903633,0.00034887006,0.00028869286,0.00030655184,0.0006094905,0.00070576195,0.00076350366,0.0004102071,0.000110893365],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003907405,0.00009922429,0.35519937,0.00017879733,0.00015179008,0.0016941911,0.0018728304,0.45219257,0.06207328,0.103664525,0.0011168164,0.02136592],"study_design_scores_gemma":[0.00003564366,0.000032111846,0.068755835,0.000028829736,0.000018486044,0.00016021448,0.00036891084,0.90710974,0.008454925,0.014171384,0.0008226165,0.00004138453],"about_ca_topic_score_codex":0.005145456,"about_ca_topic_score_gemma":0.0017335254,"teacher_disagreement_score":0.005145456,"about_ca_system_score_codex":0.00085667905,"about_ca_system_score_gemma":0.00037652534,"threshold_uncertainty_score":0.010231018},"labels":[],"label_agreement":null},{"id":"W2002635412","doi":"10.1088/0004-637x/738/1/54","title":"GALAXY FORMATION WITH SELF-CONSISTENTLY MODELED STARS AND MASSIVE BLACK HOLES. I. FEEDBACK-REGULATED STAR FORMATION AND BLACK HOLE GROWTH","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Star formation; Galaxy; Redshift; Accretion (finance); Galaxy formation and evolution; Black hole (networking); Active galactic nucleus; Structure formation","score_opus":0.008612702941092745,"score_gpt":0.18030280895474177,"score_spread":0.17169010601364904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002635412","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9357106,0.0007293122,0.04021916,0.0008416308,0.00016600254,0.0001096049,0.0013250507,0.00037883103,0.020519845],"genre_scores_gemma":[0.9873864,0.00017596355,0.008992415,0.00015628208,0.000043321845,0.00008056476,0.00034803277,0.00006659412,0.0027503776],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982893,0.00006824524,0.0000074258915,0.000023225472,0.000027949993,0.00004415784],"domain_scores_gemma":[0.99940896,0.00019095682,0.00014089569,0.00006633465,0.00006884444,0.00012399258],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003596893,0.00046783726,0.0006921666,0.00052219693,0.0004929002,0.000824186,0.0017572289,0.0013952391,0.0029123276],"category_scores_gemma":[0.0017570633,0.00036643495,0.0008834553,0.0004857511,0.0012379038,0.0006947105,0.0012187486,0.0005781992,0.00031467786],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007920689,0.00006092988,0.009739187,0.000043776625,0.000054525804,0.00015727027,0.00007873189,0.973228,0.0012897503,0.013285838,0.00044469847,0.0015381161],"study_design_scores_gemma":[0.00005675324,0.000021842483,0.0017396635,0.0000068550803,0.0000092448445,0.000019925435,0.00003243518,0.9939867,0.00014469233,0.0033964152,0.00057810405,0.0000073897063],"about_ca_topic_score_codex":0.028543346,"about_ca_topic_score_gemma":0.013157789,"teacher_disagreement_score":0.028543346,"about_ca_system_score_codex":0.0011850315,"about_ca_system_score_gemma":0.0007515043,"threshold_uncertainty_score":0.05675441},"labels":[],"label_agreement":null},{"id":"W2002786127","doi":"10.1088/0004-637x/770/2/143","title":"WIDE INTEGRAL-FIELD INFRARED SPECTROSCOPY OF THE BRIGHT [Fe II] SHELL IN THE YOUNG SUPERNOVA REMNANT G11.2–0.3","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Ejecta; Supernova remnant; Supernova; Shell (structure); Extinction (optical mineralogy); Line (geometry); Spectroscopy; Spectral line","score_opus":0.006874753259262394,"score_gpt":0.22199403920043553,"score_spread":0.21511928594117313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002786127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993765,0.00004736927,0.00015207934,0.000005456287,0.000001095449,0.0000019113443,0.000059427184,0.00001546189,0.0003408768],"genre_scores_gemma":[0.9989305,0.000046338646,0.00053205655,0.000014306348,0.0000035807063,0.0000028421098,0.0002921763,0.000006369173,0.00017170492],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999645,0.0000029869675,0.000001780466,0.000011290731,0.0000090359445,0.000010419816],"domain_scores_gemma":[0.9998803,0.00001394542,0.00003277866,0.000011577002,0.000017465622,0.000043866046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019070931,0.00022404779,0.00013382442,0.0004904608,0.00019147476,0.00022227135,0.00017100465,0.00017446297,0.00040097826],"category_scores_gemma":[0.00014664549,0.00012755067,0.00018120355,0.00021604807,0.0001377145,0.00013556187,0.0002485183,0.00015918094,0.00011793787],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005243512,0.00015408987,0.4301837,0.000055442895,0.00010042303,0.0011995921,0.00034268084,0.0013872085,0.55569845,0.00026179268,0.0004173401,0.009674892],"study_design_scores_gemma":[0.000008219806,0.00010147314,0.9906895,0.000003951089,0.000027267688,0.0004633339,0.000074488686,0.001232489,0.0070159873,0.0000454979,0.00033014285,0.0000076448705],"about_ca_topic_score_codex":0.0019146575,"about_ca_topic_score_gemma":0.0032870658,"teacher_disagreement_score":0.0019146575,"about_ca_system_score_codex":0.0001498447,"about_ca_system_score_gemma":0.00006569396,"threshold_uncertainty_score":0.0038070679},"labels":[],"label_agreement":null},{"id":"W2002836553","doi":"10.1088/0004-637x/767/2/173","title":"WEATHER ON OTHER WORLDS. I. DETECTION OF PERIODIC VARIABILITY IN THE L3 DWARF DENIS-P J1058.7-1548 WITH PRECISE MULTI-WAVELENGTH PHOTOMETRY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal; University of Toronto","funders":"","keywords":"Physics; Photometry (optics); Amplitude; Astrophysics; Rotation period; Brightness; Wavelength; Astronomy; Stars; Optics","score_opus":0.010992124732964369,"score_gpt":0.2221926481801425,"score_spread":0.21120052344717813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002836553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8809629,0.002128651,0.0012137354,0.0017266112,0.00030528544,0.000023723183,0.0041724546,0.00016092183,0.109305754],"genre_scores_gemma":[0.991028,0.0005845422,0.0005153589,0.00018607805,0.000076534474,0.0000063448006,0.0010192838,0.000019723691,0.0065641017],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999032,0.000012527338,0.0000047599137,0.000029047125,0.00002889015,0.000021609225],"domain_scores_gemma":[0.99968266,0.000039540904,0.00008472366,0.00006222615,0.00005799308,0.000072862436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013951377,0.00008761906,0.000088450746,0.0006081449,0.0006798364,0.0012057447,0.00013597422,0.00023839029,0.0052918005],"category_scores_gemma":[0.00047856427,0.0000676779,0.00009719601,0.00078072154,0.00036112173,0.0009522843,0.00078042067,0.0002736802,0.0006795135],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000576891,0.00007695758,0.7375609,0.00020699255,0.00016839085,0.001078186,0.0046927957,0.0009062377,0.028204998,0.014556234,0.02328203,0.18868944],"study_design_scores_gemma":[0.000010672962,0.0000280121,0.9033188,0.00004878637,0.00003221078,0.00032223534,0.0034817837,0.0004315427,0.0023643826,0.0023489122,0.08759585,0.000016736572],"about_ca_topic_score_codex":0.013736001,"about_ca_topic_score_gemma":0.03706373,"teacher_disagreement_score":0.013736001,"about_ca_system_score_codex":0.0003943936,"about_ca_system_score_gemma":0.00023245488,"threshold_uncertainty_score":0.0273121},"labels":[],"label_agreement":null},{"id":"W2002858718","doi":"10.1088/0004-637x/697/1/867","title":"A<i>CHANDRA</i>X-RAY ANALYSIS OF ABELL 1664: COOLING, FEEDBACK, AND STAR FORMATION IN THE CENTRAL CLUSTER GALAXY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Metallicity; Cooling flow; Star formation; Galaxy; Cluster (spacecraft); Astronomy; Luminosity; Stars","score_opus":0.00617175618412681,"score_gpt":0.20844283958795137,"score_spread":0.20227108340382458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002858718","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99087244,0.00016219284,0.00056613126,0.00010465237,0.00001723593,0.00002018889,0.0049806847,0.00025646863,0.0030200265],"genre_scores_gemma":[0.9874135,0.00012105565,0.0035284753,0.000097521,0.000038356025,0.00001543495,0.0069219912,0.00008816423,0.0017755703],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999342,0.000004091807,0.0000055910673,0.000012806943,0.000018186234,0.000025049108],"domain_scores_gemma":[0.9997491,0.00002269205,0.000082025465,0.000028863093,0.00003267739,0.00008464118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001252663,0.00029162908,0.00023826599,0.0015477504,0.00051494676,0.00053751434,0.0002903814,0.00020112551,0.0033361206],"category_scores_gemma":[0.00022166267,0.00013550023,0.0004948284,0.00080454536,0.00015626432,0.00019843229,0.00029400844,0.00032966048,0.00045807814],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009636168,0.00035747388,0.6859187,0.00023122545,0.00028695932,0.002001669,0.00046526262,0.0028155048,0.2762713,0.0010746816,0.009957796,0.019655848],"study_design_scores_gemma":[0.000007732447,0.00003590328,0.9921548,0.0000051943207,0.00001685231,0.00034598054,0.00005045999,0.0011791697,0.0041297493,0.00009582703,0.0019666003,0.000011707502],"about_ca_topic_score_codex":0.011128659,"about_ca_topic_score_gemma":0.017611763,"teacher_disagreement_score":0.011128659,"about_ca_system_score_codex":0.0003673373,"about_ca_system_score_gemma":0.00022188028,"threshold_uncertainty_score":0.022127748},"labels":[],"label_agreement":null},{"id":"W2002944265","doi":"10.1086/318688","title":"Detection of the Faint Companion in the Massive Binary HD 199579","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto; University of Victoria","funders":"","keywords":"Physics; Binary number; Astronomy; Astrophysics; Binary star; Stars","score_opus":0.011399078632801653,"score_gpt":0.22037945244306678,"score_spread":0.20898037381026513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002944265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985545,0.0001533619,0.00011735812,0.000021176067,0.000006617944,0.0000021001247,0.00008131656,0.00000676358,0.001056738],"genre_scores_gemma":[0.99904186,0.000058874804,0.0003445095,0.0000111873005,0.00001329554,0.0000021651406,0.00025460235,0.0000021959775,0.00027114403],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998783,0.000008120408,0.0000060311004,0.000029766798,0.0000508952,0.000026841124],"domain_scores_gemma":[0.9997024,0.000033238455,0.00010694914,0.000027839682,0.000031491963,0.00009813325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019587162,0.00018889307,0.0002809268,0.0007393742,0.0007923972,0.0006565208,0.00043686194,0.00038816436,0.0009628168],"category_scores_gemma":[0.00071466825,0.000112553374,0.00010064055,0.00045607978,0.0003033821,0.00021820793,0.00066224823,0.00026599254,0.0004234044],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083215785,0.00029067136,0.76739967,0.00011031452,0.000098274584,0.003892281,0.001176406,0.0013516694,0.14948013,0.0033568412,0.0023382087,0.069673374],"study_design_scores_gemma":[0.000056029694,0.00033582986,0.97542965,0.000016767937,0.00003662482,0.003316226,0.0002284768,0.0021365657,0.012375505,0.00060082716,0.0054499577,0.000017545703],"about_ca_topic_score_codex":0.002212501,"about_ca_topic_score_gemma":0.0042191385,"teacher_disagreement_score":0.002212501,"about_ca_system_score_codex":0.0004649087,"about_ca_system_score_gemma":0.00015483849,"threshold_uncertainty_score":0.0043992996},"labels":[],"label_agreement":null},{"id":"W2002969540","doi":"10.1088/0004-637x/746/2/189","title":"SIZES OF GALACTIC GLOBULAR CLUSTERS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Astrophysics; Metallicity; Physics; Luminosity; Horizontal branch; Cluster (spacecraft); Open cluster; Power law; Orbit (dynamics); Astronomy; Galaxy; Stars; Mathematics; Statistics","score_opus":0.011118672370703518,"score_gpt":0.22896595907546505,"score_spread":0.21784728670476153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2002969540","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9919962,0.00096826034,0.00044374433,0.000099411074,0.000009123104,0.000006647379,0.0016640255,0.00004696191,0.004765588],"genre_scores_gemma":[0.99742234,0.0002146049,0.000270545,0.00001918529,0.000009496266,0.0000054192474,0.0015463809,0.000026694115,0.0004853108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995977,0.000047432884,0.000024340912,0.00018217527,0.00010706825,0.000041268646],"domain_scores_gemma":[0.99760675,0.0010247094,0.00041831553,0.00021652019,0.0003977842,0.00033578541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005050472,0.000108424225,0.00020936942,0.001938513,0.00039445583,0.00090139994,0.0004947732,0.00024121645,0.0018743639],"category_scores_gemma":[0.0045886333,0.00013800028,0.0001371918,0.000975107,0.0003997106,0.0004857514,0.00055559695,0.00017645417,0.00046309308],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004645126,0.00001183563,0.9245663,0.00013592419,0.0002058459,0.00021891003,0.0018322872,0.0030115577,0.02936342,0.009470154,0.0023014052,0.02841787],"study_design_scores_gemma":[0.000007133682,0.00002847696,0.99093026,0.00000881204,0.000024128633,0.00045102584,0.00033931408,0.0011258592,0.0025503868,0.0019669144,0.0025537699,0.000013932164],"about_ca_topic_score_codex":0.004399973,"about_ca_topic_score_gemma":0.003972402,"teacher_disagreement_score":0.004399973,"about_ca_system_score_codex":0.00075356074,"about_ca_system_score_gemma":0.00026216582,"threshold_uncertainty_score":0.00874877},"labels":[],"label_agreement":null},{"id":"W2003010321","doi":"10.1088/0004-637x/710/2/1868","title":"ERRATUM: “H I CLOUDS IN THE LOWER HALO. I. THE GALACTIC ALL-SKY SURVEY PILOT REGION” (2008, ApJ, 688, 290)","year":2010,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Sky; Halo; Astrophysics; Galactic halo; Astronomy; Galaxy","score_opus":0.032528940560959195,"score_gpt":0.26056799831947863,"score_spread":0.22803905775851943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003010321","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0014552003,0.0021732952,0.0008676645,0.047087494,0.926521,0.000042471267,0.01083365,0.0010288002,0.009990464],"genre_scores_gemma":[0.049039543,0.018293317,0.016508844,0.12905401,0.20878612,0.0005142258,0.07791949,0.007816023,0.4920684],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9984068,0.00014976999,0.00031605354,0.00022285421,0.0007906197,0.0001139164],"domain_scores_gemma":[0.9899149,0.0011034106,0.00088726793,0.0007667753,0.0067396415,0.00058798044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021647091,0.0018779543,0.0011258969,0.0035165593,0.0039664973,0.0028726372,0.0019329893,0.0027835537,0.034609716],"category_scores_gemma":[0.018278575,0.00092085835,0.0011149627,0.0037964624,0.0013670888,0.0020252485,0.0020800103,0.005100312,0.044041038],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027265725,0.000005824167,0.00024440803,0.000049622362,0.000005211438,0.00009767445,0.000024594809,0.000019636836,0.00004516875,0.00031122658,0.99489284,0.0042765792],"study_design_scores_gemma":[0.00003882595,0.000030432437,0.0044886116,0.00029622295,0.000038830913,0.00036969842,0.00019811992,0.000108861626,0.00043288147,0.00046830135,0.9934849,0.00004431463],"about_ca_topic_score_codex":0.061418157,"about_ca_topic_score_gemma":0.058455434,"teacher_disagreement_score":0.061418157,"about_ca_system_score_codex":0.00335352,"about_ca_system_score_gemma":0.005084934,"threshold_uncertainty_score":0.122121334},"labels":[],"label_agreement":null},{"id":"W2003018282","doi":"10.1088/0004-637x/719/2/1104","title":"A NEW SAMPLE OF VERY MASSIVE STAR FORMING COMPLEXES IN THE<i>SPITZER</i>GLIMPSE SURVEY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"CMB cold spot; Star formation; Kinetic energy; Bubble; Star (game theory); Luminosity; Line (geometry); Radial velocity; Proper motion","score_opus":0.02068684798007506,"score_gpt":0.2847913656452033,"score_spread":0.2641045176651282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003018282","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99912983,0.000041703577,0.00009003635,0.000016519862,9.4089233e-7,0.000011981833,0.00045964716,0.0000071110826,0.00024225297],"genre_scores_gemma":[0.99571395,0.00012147276,0.0005576169,0.000052340485,0.000012306351,0.000031873948,0.0029686748,0.0000136119925,0.0005280325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979585,0.000017138596,0.00001641835,0.000056907884,0.00006229454,0.000051327628],"domain_scores_gemma":[0.9993789,0.000050165054,0.0001848962,0.00007194947,0.000074647985,0.00023932457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028435144,0.00033265693,0.00034246332,0.0018984338,0.00040359522,0.00058912515,0.00039525307,0.0002016303,0.0011030907],"category_scores_gemma":[0.0006630708,0.00023883276,0.0002692452,0.0008974997,0.00028913413,0.00050963694,0.00093027216,0.00026848668,0.0004089742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008261031,0.000043624546,0.9896841,0.000011669053,0.000041207993,0.00025120456,0.0006455525,0.00005683233,0.004508265,0.00006009409,0.0005335567,0.0040813177],"study_design_scores_gemma":[0.0000041615776,0.000025184103,0.99860746,0.0000018352437,0.000008190948,0.00024627158,0.00016732475,0.000074149844,0.00015043044,0.00001134063,0.00070146745,0.0000021888832],"about_ca_topic_score_codex":0.0077911234,"about_ca_topic_score_gemma":0.0141009595,"teacher_disagreement_score":0.0077911234,"about_ca_system_score_codex":0.00022832245,"about_ca_system_score_gemma":0.00019832143,"threshold_uncertainty_score":0.015491545},"labels":[],"label_agreement":null},{"id":"W2003110711","doi":"10.1086/427720","title":"The Acceleration Mechanism of Resistive Magnetohydrodynamic Jets Launched from Accretion Disks","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Magnetohydrodynamics; Magnetohydrodynamic drive; Torus; Mechanics; Magnetic field; RADIUS; Field line; Jet (fluid); Acceleration; Angular momentum; Classical mechanics; Geometry","score_opus":0.011487823445028036,"score_gpt":0.23266484989871788,"score_spread":0.22117702645368986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003110711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939732,0.000100391786,0.0032776173,0.00010320161,0.000012413346,0.000015915628,0.000059464335,0.00006542375,0.0023923323],"genre_scores_gemma":[0.99893075,0.00003871511,0.0006667833,0.000007843414,0.0000059650083,0.0000071389286,0.000038795162,0.000011173944,0.00029277997],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989355,0.000030039399,0.0000051926368,0.000012472298,0.000021483182,0.000037226102],"domain_scores_gemma":[0.99956685,0.00017339684,0.00008945679,0.00003607927,0.00005432104,0.00007981432],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024386913,0.0005022096,0.0003524986,0.00034633712,0.00043389574,0.0006522935,0.0006852288,0.0005593243,0.0007856157],"category_scores_gemma":[0.0015350787,0.00029280028,0.00037368483,0.00026653783,0.0005289521,0.0005594328,0.00044864372,0.0003842527,0.00011470805],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003506991,0.00010138069,0.015584798,0.00008480518,0.00006867497,0.0011518308,0.00027304166,0.9466426,0.02635819,0.00580658,0.00035887616,0.0032185258],"study_design_scores_gemma":[0.000047790913,0.000054529613,0.0039754915,0.0000032526186,0.000011342518,0.00004925067,0.00003317731,0.99257493,0.002188112,0.0008652868,0.00018709828,0.000009713601],"about_ca_topic_score_codex":0.0032788664,"about_ca_topic_score_gemma":0.0009326471,"teacher_disagreement_score":0.0032788664,"about_ca_system_score_codex":0.0005336969,"about_ca_system_score_gemma":0.00024317186,"threshold_uncertainty_score":0.006519556},"labels":[],"label_agreement":null},{"id":"W2003136270","doi":"10.1086/379309","title":"Spontaneous Generation of the Magnetic Field and Suppression of the Heat Conduction in Cold Fronts","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Magnetic field; Instability; Thermal conduction; Electron; Condensed matter physics; Plasma; Saturation (graph theory); Anisotropy; Mechanics; Optics","score_opus":0.010972839101281153,"score_gpt":0.217817142551245,"score_spread":0.20684430344996385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003136270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99549234,0.00025588123,0.002937258,0.000022863218,0.000007909443,0.0000071739096,0.000028072665,0.00003635597,0.0012120333],"genre_scores_gemma":[0.9986085,0.000050331455,0.00058729853,0.000006595707,0.000009420859,0.0000052742007,0.000042147858,0.000007156684,0.00068323564],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994564,0.0000060717666,0.0000019495553,0.000007784951,0.000013061456,0.000025462461],"domain_scores_gemma":[0.99972004,0.00004779375,0.00006842998,0.000047769416,0.000066961504,0.000048947677],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013287978,0.00016992261,0.00021045942,0.0003834201,0.00037733364,0.0005231475,0.00028715126,0.00019924562,0.0010149746],"category_scores_gemma":[0.0004309548,0.00012657435,0.0002290839,0.00011165436,0.00040815148,0.0002718846,0.0004162498,0.0002543331,0.00023614615],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030612404,0.000042776996,0.0093154805,0.000058786914,0.000011847574,0.00026203136,0.00026451124,0.0014511986,0.9771418,0.0056722523,0.00013145265,0.005341753],"study_design_scores_gemma":[0.000114947,0.00040469566,0.07155197,0.000021095295,0.000048035585,0.0009156892,0.00022937398,0.035447594,0.88004524,0.007223854,0.0039623505,0.000035096764],"about_ca_topic_score_codex":0.0005066671,"about_ca_topic_score_gemma":0.00037478865,"teacher_disagreement_score":0.0010149746,"about_ca_system_score_codex":0.00024299294,"about_ca_system_score_gemma":0.00013595594,"threshold_uncertainty_score":0.0033954382},"labels":[],"label_agreement":null},{"id":"W2003164007","doi":"10.1086/382147","title":"The<i>s</i>‐Process in Metal‐Poor Stars: Abundances for 22 Neutron‐Capture Elements in CS 31062‐050","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Stellar atmosphere; Spectral line; Astronomical spectroscopy; Abundance (ecology); Background radiation; Stellar evolution","score_opus":0.009543209277321546,"score_gpt":0.25009697228609423,"score_spread":0.24055376300877268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003164007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936701,0.00012602501,0.00018828725,0.000044811324,0.000009796662,0.0000065403083,0.00045175944,0.00003180209,0.0054708146],"genre_scores_gemma":[0.994167,0.00007732499,0.00029148796,0.000055340734,0.000007252793,0.0000046908226,0.0008568938,0.000024989573,0.0045150393],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999037,0.0000066800517,0.000005870843,0.000032552824,0.000027766238,0.00002341637],"domain_scores_gemma":[0.99959046,0.00008555683,0.000085838205,0.000028129796,0.0001159535,0.000094105424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003235842,0.00031305425,0.00021833011,0.001325353,0.00074846647,0.0007686763,0.00031839483,0.00040310458,0.0040368238],"category_scores_gemma":[0.00061039825,0.0002084112,0.00015583816,0.0006603572,0.00038435438,0.000458385,0.00042736533,0.00026144396,0.00074281683],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024336623,0.000208501,0.6187685,0.00018124092,0.00008060046,0.0007932231,0.00064904377,0.0024668481,0.33899182,0.003076449,0.0028565172,0.029493537],"study_design_scores_gemma":[0.000075413715,0.00032098207,0.9327213,0.000021928878,0.000050356568,0.00056102255,0.0004591448,0.003936171,0.053841043,0.00080619234,0.007183818,0.000022631126],"about_ca_topic_score_codex":0.008485961,"about_ca_topic_score_gemma":0.012481744,"teacher_disagreement_score":0.008485961,"about_ca_system_score_codex":0.00068577466,"about_ca_system_score_gemma":0.0004034362,"threshold_uncertainty_score":0.01687318},"labels":[],"label_agreement":null},{"id":"W2003223986","doi":"10.1086/309332","title":"Extended X‐Ray Emission from the Planetary Nebula BD +30o3639","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Planetary nebula; ROSAT; Nebula; Astrophysics; Emission nebula; Astronomy; Hubble space telescope; Spitzer Space Telescope; Protoplanetary nebula; Wolf–Rayet star; Reflection nebula; Telescope; Stars; Galaxy","score_opus":0.007994958054330547,"score_gpt":0.22022993750615089,"score_spread":0.21223497945182035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003223986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954917,0.00030883725,0.00018646198,0.000042927335,0.000010476666,0.000007855435,0.000845943,0.000015927286,0.003089812],"genre_scores_gemma":[0.9966126,0.00025971286,0.0005000752,0.0000399204,0.000010200104,0.0000050117283,0.0018071249,0.0000066208086,0.00075869705],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998753,0.000005255038,0.0000054577454,0.000030791518,0.000047484347,0.000035674973],"domain_scores_gemma":[0.9998647,0.0000075286353,0.000027495542,0.000016531443,0.000012299839,0.00007139626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001188666,0.0001998886,0.0002610173,0.0004059629,0.0005754061,0.0005250326,0.00023005113,0.00024571762,0.0024266692],"category_scores_gemma":[0.00017573452,0.00014677097,0.00014165942,0.0005287545,0.0003001699,0.00017275728,0.0007798125,0.0002556569,0.00081900007],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083993963,0.00018065175,0.4353847,0.00019632015,0.00006793999,0.003578887,0.0008577946,0.0006593274,0.51750445,0.0012578535,0.0024237358,0.037048552],"study_design_scores_gemma":[0.00003936276,0.00018884307,0.96696246,0.00002282365,0.000020247378,0.0047012344,0.000219915,0.00046312803,0.009790129,0.00049407664,0.017072728,0.000024985206],"about_ca_topic_score_codex":0.005017516,"about_ca_topic_score_gemma":0.007271023,"teacher_disagreement_score":0.005017516,"about_ca_system_score_codex":0.00028773825,"about_ca_system_score_gemma":0.00020795784,"threshold_uncertainty_score":0.009976625},"labels":[],"label_agreement":null},{"id":"W2003234024","doi":"10.1088/0004-637x/737/2/92","title":"KECK DEEP FIELDS. IV. LUMINOSITY-DEPENDENT CLUSTERING AND GALAXY DOWNSIZING IN UV-SELECTED GALAXIES AT<i>z</i>= 4, 3, AND 2","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Galaxy; Halo; Dark matter; Luminosity; Redshift; Cluster analysis; Stellar mass; Galaxy formation and evolution","score_opus":0.010248035893542009,"score_gpt":0.19696854956346205,"score_spread":0.18672051366992004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003234024","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973544,0.00003353179,0.0001769184,0.000019540894,0.0000016559209,0.0000045370994,0.0014600976,0.000016987155,0.00093232916],"genre_scores_gemma":[0.9958456,0.000022476066,0.00050987914,0.00001677786,0.0000025918403,0.0000068018185,0.00287634,0.0000071176746,0.00071245787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989617,0.000009505903,0.0000046582454,0.000032576554,0.000014841546,0.000042248957],"domain_scores_gemma":[0.99916434,0.00012097211,0.0003194597,0.000106994376,0.000076073244,0.00021219505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000290217,0.00019155565,0.00017469635,0.001023545,0.00026708274,0.00032139334,0.0002582466,0.00016108266,0.0018982748],"category_scores_gemma":[0.0007295593,0.00015508423,0.00020634671,0.0006410412,0.00025495587,0.00043432444,0.00043511117,0.00031501497,0.00032888295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034564958,0.000087743065,0.98261225,0.000027581264,0.00005463622,0.0001077626,0.00020058862,0.0023030434,0.006889749,0.00066003186,0.0012507424,0.0054602814],"study_design_scores_gemma":[0.0000063583097,0.000015578195,0.997591,0.000002835004,0.0000053901167,0.00004810243,0.000060810067,0.0010507845,0.0007423788,0.00011097876,0.0003625894,0.000003286505],"about_ca_topic_score_codex":0.014067172,"about_ca_topic_score_gemma":0.025602438,"teacher_disagreement_score":0.014067172,"about_ca_system_score_codex":0.00060006924,"about_ca_system_score_gemma":0.0001357184,"threshold_uncertainty_score":0.027970612},"labels":[],"label_agreement":null},{"id":"W2003236043","doi":"10.1088/0004-637x/721/2/1113","title":"THE MECHANICAL GREENHOUSE: BURIAL OF HEAT BY TURBULENCE IN HOT JUPITER ATMOSPHERES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Hot Jupiter; Turbulence; Heat flux; Radiative cooling; Convection; Mixing (physics); Planet; Jupiter (rocket family); Convective heat transfer","score_opus":0.005970839979891056,"score_gpt":0.21507569517220632,"score_spread":0.20910485519231525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003236043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925783,0.0007737025,0.0022103651,0.00075630745,0.000048911625,0.000011522978,0.00006061262,0.000167909,0.0033924035],"genre_scores_gemma":[0.99951684,0.0000704907,0.00014312527,0.000033956996,0.000023872828,0.000002336791,0.000013771634,0.000011142341,0.00018443841],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999454,0.0000107212945,0.0000027712858,0.000009529926,0.000008159637,0.000023555256],"domain_scores_gemma":[0.99986565,0.00003198512,0.0000380148,0.000014898171,0.000009148583,0.000040263825],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015851494,0.00036838837,0.0002835209,0.0003252801,0.0005096897,0.00067984936,0.00030401014,0.00041866736,0.0016530827],"category_scores_gemma":[0.00040836612,0.00019511521,0.00034139885,0.000116883886,0.0006487107,0.00083828054,0.0007055885,0.00032784924,0.000119294236],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015796722,0.00052449,0.16507241,0.0004446809,0.00030514313,0.0032410948,0.0013863115,0.07695125,0.65401345,0.06332511,0.004123147,0.029033283],"study_design_scores_gemma":[0.00037213523,0.0008827909,0.5062418,0.00007004768,0.00018251983,0.0006925105,0.00061966584,0.40615878,0.047258165,0.03222009,0.00512893,0.00017253],"about_ca_topic_score_codex":0.0019243931,"about_ca_topic_score_gemma":0.00094604975,"teacher_disagreement_score":0.0019243931,"about_ca_system_score_codex":0.00042596235,"about_ca_system_score_gemma":0.00015729867,"threshold_uncertainty_score":0.0055300593},"labels":[],"label_agreement":null},{"id":"W2003246823","doi":"10.1086/510306","title":"Propagation of the First Flames in Type Ia Supernovae","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Laminar flow; Supernova; Buoyancy; Astrophysics; Physics; White dwarf; Mechanics; Turbulence; Thermonuclear fusion; Ignition system; Flame speed; Combustion; Diffusion flame; Combustor; Chemistry; Stars; Thermodynamics; Plasma; Nuclear physics","score_opus":0.009446610112847115,"score_gpt":0.23646882605822842,"score_spread":0.2270222159453813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003246823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9301993,0.00088811066,0.05691854,0.00020798219,0.0001266023,0.000073890005,0.0001499945,0.00025687343,0.011178753],"genre_scores_gemma":[0.9911146,0.00033421317,0.0060647614,0.000021542186,0.000020263082,0.000027865912,0.00006864241,0.000049997838,0.0022980128],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994063,0.000011255757,0.0000024728777,0.000008354094,0.000016312812,0.000020961208],"domain_scores_gemma":[0.999635,0.00007565454,0.00013034401,0.000018602977,0.00004914627,0.00009124383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032977428,0.00058488373,0.0002665732,0.0005342168,0.0006571969,0.00096979825,0.0005241535,0.00062971713,0.0012765045],"category_scores_gemma":[0.0011405553,0.0003015852,0.00055732124,0.00021031058,0.00083334104,0.00065001374,0.0011763788,0.0006345659,0.00015805506],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029349764,0.00015954116,0.01505281,0.00011590639,0.00006665231,0.00080131536,0.00059655966,0.8408064,0.020068629,0.11305414,0.00061649806,0.008367986],"study_design_scores_gemma":[0.000040619016,0.000083886254,0.00347645,0.000022920347,0.000017765724,0.000094512136,0.00010350334,0.98084027,0.0025010682,0.011681682,0.0011117358,0.000025599824],"about_ca_topic_score_codex":0.0121959075,"about_ca_topic_score_gemma":0.0037217988,"teacher_disagreement_score":0.0121959075,"about_ca_system_score_codex":0.0009946603,"about_ca_system_score_gemma":0.00051922543,"threshold_uncertainty_score":0.024249852},"labels":[],"label_agreement":null},{"id":"W2003247943","doi":"10.1086/588646","title":"The Nonlinear Evolution of Galaxy Intrinsic Alignments","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Halo; Redshift; Nonlinear system; Galaxy; Spin (aerodynamics); Angular momentum; Halo effect; Tidal force; Gravitation","score_opus":0.007061706820254755,"score_gpt":0.2305420149070119,"score_spread":0.22348030808675715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003247943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9871803,0.00006122944,0.009683772,0.00007667971,0.0000052194637,0.000007185111,0.00009290438,0.000085242544,0.0028075692],"genre_scores_gemma":[0.99885917,0.000032938307,0.00069922017,0.0000047416574,0.0000030966098,0.0000026194762,0.000037331643,0.000014460735,0.0003463978],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998939,0.000023762379,0.000005504668,0.000023700773,0.000027370423,0.000025683044],"domain_scores_gemma":[0.9992048,0.00022402934,0.00025657305,0.000109915236,0.000107752276,0.00009692846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003323944,0.00030537279,0.00020045621,0.00044063418,0.00033100176,0.0006363283,0.00030065677,0.00022351096,0.0012799156],"category_scores_gemma":[0.002846034,0.00030501984,0.00034156686,0.00036146617,0.00055966293,0.00066633103,0.00055279495,0.00034115353,0.0001221238],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013447071,0.000041106952,0.14522918,0.00006479464,0.00009413235,0.0004987167,0.00026269024,0.7871973,0.02841895,0.029803133,0.00048122305,0.007774297],"study_design_scores_gemma":[0.00000891016,0.00001927122,0.03350292,0.000003169042,0.000013707473,0.000056694444,0.000022694576,0.9611658,0.0021755255,0.0028357795,0.00018159687,0.000014019989],"about_ca_topic_score_codex":0.0067541385,"about_ca_topic_score_gemma":0.0058793826,"teacher_disagreement_score":0.0067541385,"about_ca_system_score_codex":0.00087605434,"about_ca_system_score_gemma":0.0004060169,"threshold_uncertainty_score":0.013429642},"labels":[],"label_agreement":null},{"id":"W2003269131","doi":"10.1086/343030","title":"Cataclysmic Variables: An Empirical Angular Momentum Loss Prescription from Open Cluster Data","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Angular momentum; Physics; Astrophysics; Specific relative angular momentum; Accretion (finance); Stars; Total angular momentum quantum number; Classical mechanics; Angular momentum coupling","score_opus":0.045590725158908614,"score_gpt":0.3024394625246803,"score_spread":0.2568487373657717,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003269131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900075,0.00017238558,0.007728626,0.0000664271,0.0000073767355,0.00001755772,0.0005092776,0.000089180096,0.0014015376],"genre_scores_gemma":[0.996923,0.000050847182,0.002279928,0.000009505935,0.0000069968673,0.000009835944,0.0005941002,0.000022613774,0.00010305784],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997085,0.00006629786,0.000028555662,0.0000952423,0.00006384473,0.000037424332],"domain_scores_gemma":[0.99675214,0.0011897786,0.0008987578,0.0007197938,0.0002790628,0.00016043364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013910738,0.0002586083,0.00018317837,0.0010971266,0.00037487637,0.00093648577,0.00059767964,0.00027594418,0.00046279014],"category_scores_gemma":[0.0063195126,0.00011550226,0.00023112203,0.0011073131,0.00036076418,0.00060620887,0.00075160427,0.00047543875,0.0001550273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016519903,0.000031710555,0.9428661,0.00006369098,0.00006656508,0.00014099113,0.0003120347,0.026260026,0.0031553304,0.002881621,0.00058011076,0.023476673],"study_design_scores_gemma":[0.0000269437,0.000094312294,0.8162642,0.00003414729,0.00004030401,0.00028628175,0.00019727883,0.17226371,0.0031945126,0.004928901,0.0026369751,0.00003232378],"about_ca_topic_score_codex":0.0048884065,"about_ca_topic_score_gemma":0.0032078335,"teacher_disagreement_score":0.0048884065,"about_ca_system_score_codex":0.00049364264,"about_ca_system_score_gemma":0.00029527448,"threshold_uncertainty_score":0.009719908},"labels":[],"label_agreement":null},{"id":"W2003357980","doi":"10.1086/503546","title":"Optical Detection of Two Intermediate-Mass Binary Pulsar Companions","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Pulsar; White dwarf; Physics; Neutron star; Astrophysics; Millisecond pulsar; Chandrasekhar limit; Binary pulsar; Astronomy; Binary number; Stars","score_opus":0.00919094755227658,"score_gpt":0.30193232599570413,"score_spread":0.29274137844342757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003357980","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99762267,0.00022847875,0.00038614645,0.000031977288,0.000010051377,0.000006234926,0.00004818196,0.000023595849,0.0016425677],"genre_scores_gemma":[0.99908113,0.000050404524,0.0005239567,0.00002665104,0.000013205028,0.0000033341498,0.000095341326,0.0000017743661,0.00020407839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998429,0.00000989262,0.000009190953,0.000052456275,0.000040110604,0.000045374094],"domain_scores_gemma":[0.999648,0.000047387697,0.00011461499,0.000041125862,0.000038479622,0.00011040069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017005975,0.00018614429,0.00016734115,0.00062099996,0.0004305466,0.0005661371,0.00026059186,0.0004720476,0.0014382416],"category_scores_gemma":[0.0005341119,0.00015376914,0.00008741401,0.00028134976,0.0002981474,0.00023524885,0.0006231225,0.00032599666,0.00024400563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045707004,0.00029271372,0.69720894,0.00012335154,0.00008743581,0.004839401,0.00075628737,0.00019077568,0.24799852,0.0011695235,0.0007277002,0.046148352],"study_design_scores_gemma":[0.00006469539,0.00085340475,0.9183073,0.000018369103,0.00010364522,0.019682223,0.000352343,0.0008707779,0.05181171,0.0008496699,0.0070656557,0.000020006271],"about_ca_topic_score_codex":0.0004361061,"about_ca_topic_score_gemma":0.00058731507,"teacher_disagreement_score":0.0014382416,"about_ca_system_score_codex":0.00011106778,"about_ca_system_score_gemma":0.000106484404,"threshold_uncertainty_score":0.0048113465},"labels":[],"label_agreement":null},{"id":"W2003412632","doi":"10.1088/0004-637x/709/1/332","title":"SIMULTANEOUS MULTI-WAVELENGTH OBSERVATIONS OF MAGNETIC ACTIVITY IN ULTRACOOL DWARFS. III. X-RAY, RADIO, AND Hα ACTIVITY TRENDS IN M AND L DWARFS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Luminosity; Brown dwarf; Stellar classification; H-alpha; Astronomy; Spectral line; Stars; Emission spectrum; Galaxy","score_opus":0.01758879579480669,"score_gpt":0.24281506936287872,"score_spread":0.22522627356807204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003412632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99916995,0.00010664078,0.00009722198,0.000008050094,0.0000012567906,0.0000024218853,0.00018340268,0.000012880698,0.00041819277],"genre_scores_gemma":[0.9982584,0.0000780624,0.00053923344,0.000035446028,0.000009149953,0.000007660779,0.00065726176,0.0000062528375,0.00040856455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988675,0.000010463417,0.000008970771,0.000034528966,0.000026374359,0.000032919408],"domain_scores_gemma":[0.9994289,0.000051357845,0.0001984283,0.000038766862,0.0000758807,0.00020661516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021577429,0.00017439178,0.00022032614,0.0012615528,0.00036569982,0.00034642252,0.00026184582,0.0001915288,0.00054094533],"category_scores_gemma":[0.00037978965,0.00017305618,0.00015792417,0.00059712474,0.00018565152,0.00021163297,0.0005547606,0.00024836857,0.00029725084],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030168437,0.00006409176,0.86816365,0.000047071764,0.00004471412,0.00018372975,0.00084442936,0.00011296797,0.1170893,0.000049265433,0.00021561643,0.012883515],"study_design_scores_gemma":[0.0000047573826,0.000058393132,0.99761945,0.0000035337855,0.000007719609,0.00014632048,0.00013601188,0.00006420519,0.0016157164,0.0000111798345,0.0003297575,0.0000028371132],"about_ca_topic_score_codex":0.0035250946,"about_ca_topic_score_gemma":0.009786154,"teacher_disagreement_score":0.0035250946,"about_ca_system_score_codex":0.00021036311,"about_ca_system_score_gemma":0.00009068437,"threshold_uncertainty_score":0.007009208},"labels":[],"label_agreement":null},{"id":"W2003658876","doi":"10.1086/533580","title":"<i>FUSE</i>Determination of Abundances in Long‐Period Pulsating V1093 Her (PG 1716+426) Stars1","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Canadian Space Agency; Université de Montréal","funders":"","keywords":"Physics; Stars; Astrophysics; Subdwarf; Luminosity; Spectral line; Period (music); Homogeneous; Astronomy; White dwarf; Galaxy; Thermodynamics","score_opus":0.012336331143478128,"score_gpt":0.2337786049995575,"score_spread":0.22144227385607937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003658876","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808633,0.00017788583,0.00017388795,0.000009884539,0.0000017997994,0.0000018204453,0.00044211248,0.000019025278,0.001087341],"genre_scores_gemma":[0.9976284,0.00006888668,0.0005584168,0.000012008053,0.000004151511,0.0000019650092,0.0014788172,0.000006891582,0.00024041612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.000005316948,0.0000045475317,0.000019564559,0.000018947978,0.000014186495],"domain_scores_gemma":[0.99978,0.000028755758,0.00009002726,0.000024393341,0.000029873354,0.00004690783],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012647579,0.00016928658,0.00014188909,0.0009900635,0.00034868537,0.00031243256,0.000118882585,0.00023833028,0.0007100736],"category_scores_gemma":[0.00023546742,0.00006527016,0.00013320975,0.00076979893,0.0001485219,0.00019342662,0.00023539377,0.00013330136,0.00026662755],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049765216,0.00005216322,0.7933973,0.000043113057,0.0000735954,0.00035091658,0.00028041695,0.000785857,0.1870762,0.00024450288,0.00039958346,0.016798638],"study_design_scores_gemma":[0.0000022664588,0.000044230717,0.9924712,0.0000018744572,0.000009973094,0.00036465348,0.000058711015,0.0004045352,0.0058481125,0.00005701706,0.0007336932,0.0000037920186],"about_ca_topic_score_codex":0.0017452285,"about_ca_topic_score_gemma":0.002503911,"teacher_disagreement_score":0.0017452285,"about_ca_system_score_codex":0.00023943286,"about_ca_system_score_gemma":0.00005418329,"threshold_uncertainty_score":0.0034701228},"labels":[],"label_agreement":null},{"id":"W2003666254","doi":"10.1088/0004-637x/700/1/63","title":"NUMERICAL TESTS OF FAST RECONNECTION IN WEAKLY STOCHASTIC MAGNETIC FIELDS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":363,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Magnetic reconnection; Turbulence; Outflow; Mechanics; Statistical physics; Inflow; Magnetic flux; Computational physics; Magnetic field; Meteorology; Quantum mechanics","score_opus":0.005169028948516194,"score_gpt":0.22230001952090309,"score_spread":0.21713099057238688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003666254","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926057,0.00016260055,0.003728979,0.00024919995,0.000032747048,0.000019940493,0.0002576944,0.00013506747,0.0028079897],"genre_scores_gemma":[0.997698,0.000052320687,0.0018748385,0.000030180101,0.000007314954,0.000014163487,0.00010995817,0.000019030085,0.00019413466],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99969506,0.00010023651,0.000022500053,0.00003917599,0.00006209562,0.00008096262],"domain_scores_gemma":[0.9944132,0.0036051818,0.0009322996,0.0003369575,0.00033934324,0.00037296],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007499069,0.0006108711,0.0007647845,0.00076210464,0.0005771632,0.0008956357,0.0012597308,0.0011230626,0.0018022517],"category_scores_gemma":[0.0056966734,0.00030130555,0.0007055763,0.000674472,0.001203305,0.0006712826,0.0009812359,0.001123178,0.00009060052],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015350494,0.00012592676,0.008231802,0.000060130536,0.00005565023,0.00017312469,0.000090481415,0.9831441,0.0029688843,0.0037221215,0.00021742572,0.0010568765],"study_design_scores_gemma":[0.000027207636,0.000056514575,0.00084561406,0.0000058955115,0.0000059617073,0.000014185228,0.000024368912,0.99701536,0.0010050788,0.0009176158,0.00007473368,0.0000075757935],"about_ca_topic_score_codex":0.009438411,"about_ca_topic_score_gemma":0.004761934,"teacher_disagreement_score":0.009438411,"about_ca_system_score_codex":0.00084456394,"about_ca_system_score_gemma":0.00054506416,"threshold_uncertainty_score":0.018767},"labels":[],"label_agreement":null},{"id":"W2003679311","doi":"10.1086/592237","title":"Models for the Observable System Parameters of Ultraluminous X‐Ray Sources","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Galaxy; Luminosity; Black hole (networking); Observable; Accretion (finance); Binary number; Flux (metallurgy); Supermassive black hole","score_opus":0.03741095884805295,"score_gpt":0.22284753045334268,"score_spread":0.18543657160528973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003679311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97961926,0.00014795052,0.017266067,0.00013973782,0.0000072917333,0.000025360907,0.00038386844,0.000085231484,0.0023252212],"genre_scores_gemma":[0.99383,0.00012192182,0.0044738194,0.000024961026,0.000007990609,0.00006904361,0.0004947355,0.00004017749,0.0009373249],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998468,0.0000417267,0.0000071593836,0.000048762056,0.000019642237,0.000035879562],"domain_scores_gemma":[0.9991025,0.00044553497,0.0002051476,0.00008753523,0.0000729125,0.00008652919],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003964595,0.00041995905,0.0004322166,0.0005743103,0.00064695696,0.0011518883,0.0015597555,0.000868628,0.0022382587],"category_scores_gemma":[0.0023880226,0.00033941164,0.00065594976,0.0005359095,0.00050603313,0.0013379921,0.00061708095,0.0005474868,0.00028119236],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000738483,0.00005133252,0.047653012,0.00003223942,0.000054994234,0.0001642091,0.0002182553,0.9369569,0.0019345543,0.010080283,0.00031393414,0.0024664213],"study_design_scores_gemma":[0.000033575172,0.00002991046,0.010030495,0.000007850132,0.000020683998,0.00013178626,0.00007029438,0.9833309,0.00047659475,0.0053279884,0.0005273165,0.00001272104],"about_ca_topic_score_codex":0.0067429966,"about_ca_topic_score_gemma":0.005575485,"teacher_disagreement_score":0.0067429966,"about_ca_system_score_codex":0.0013553131,"about_ca_system_score_gemma":0.0004794526,"threshold_uncertainty_score":0.013407469},"labels":[],"label_agreement":null},{"id":"W2003702841","doi":"10.1088/0004-637x/762/1/57","title":"THE NEWLY DISCOVERED PULSATING LOW-MASS WHITE DWARFS: AN EXTENSION OF THE ZZ CETI INSTABILITY STRIP","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Instability strip; Physics; White dwarf; Convection; Astrophysics; Stars; Instability; Hertzsprung–Russell diagram; Low Mass; Effective temperature; Convection zone; Thermal; Stellar evolution; Astronomy; Mechanics; Thermodynamics","score_opus":0.01340205573144587,"score_gpt":0.23509520037596648,"score_spread":0.2216931446445206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003702841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9867662,0.0005057754,0.0011325504,0.00033411582,0.000040107378,0.000012826155,0.00009909058,0.000045793928,0.011063583],"genre_scores_gemma":[0.9976472,0.00014018518,0.0003612282,0.00009029835,0.00006966798,0.0000028049888,0.000105843275,0.000012590116,0.0015702752],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998246,0.0000120178465,0.000018246501,0.000045561712,0.000059684935,0.000039864168],"domain_scores_gemma":[0.9988249,0.00026574935,0.00039706394,0.00016786117,0.00019591357,0.00014846835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055834046,0.00015728411,0.00026327095,0.0011015313,0.00057483383,0.0012876783,0.0004388399,0.00040511685,0.0018692903],"category_scores_gemma":[0.0018896466,0.00011347997,0.00013331484,0.0009153717,0.00066461705,0.00055083213,0.000692412,0.00042469005,0.00052571186],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096249115,0.00012521465,0.7249938,0.00015760619,0.000056421544,0.015191416,0.0031885349,0.0002962025,0.11615015,0.011489466,0.0026372722,0.12475139],"study_design_scores_gemma":[0.00005818303,0.00030894426,0.922147,0.000038800415,0.000050217168,0.026320625,0.0012026677,0.0010147587,0.017104955,0.005442859,0.026285255,0.00002578692],"about_ca_topic_score_codex":0.000354769,"about_ca_topic_score_gemma":0.00034688914,"teacher_disagreement_score":0.0018692903,"about_ca_system_score_codex":0.00021137968,"about_ca_system_score_gemma":0.00022228259,"threshold_uncertainty_score":0.0062534213},"labels":[],"label_agreement":null},{"id":"W2003736177","doi":"10.1086/427628","title":"<i>Chandra</i> X-Ray Detection of the High Magnetic Field Radio Pulsar PSR J1718-3718","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Pulsar; Millisecond pulsar; Luminosity; X-ray pulsar; Magnetic field; Population; Magnetic dipole; Neutron star","score_opus":0.005314876232844257,"score_gpt":0.25227677681111543,"score_spread":0.24696190057827117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003736177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98725617,0.0017663594,0.0008770396,0.00035053174,0.00008895117,0.0000392828,0.0018560564,0.00019329699,0.0075723487],"genre_scores_gemma":[0.9851318,0.0016968104,0.0054067443,0.00036760283,0.00021375719,0.00003992716,0.0045239152,0.00005887698,0.002560611],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99986744,0.00000705098,0.000009796237,0.00002521482,0.000046289886,0.000044262677],"domain_scores_gemma":[0.99952996,0.00003495894,0.00016489976,0.000084559295,0.00006108161,0.00012454517],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001634298,0.00047706827,0.00028614007,0.0012317137,0.0005695965,0.000809622,0.0005507418,0.00031586483,0.00206796],"category_scores_gemma":[0.0003479465,0.0001805523,0.00018484978,0.00085437077,0.00052959303,0.000317705,0.0007315135,0.0004586818,0.0007144998],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094735896,0.00031172493,0.4409618,0.00070842414,0.00029872952,0.008934027,0.00069463253,0.00046487423,0.45015782,0.0026900356,0.017082946,0.07674765],"study_design_scores_gemma":[0.0001361905,0.0005999324,0.8358366,0.00009558231,0.00029674376,0.018397236,0.00032765992,0.0004945475,0.07911692,0.0012217105,0.06341189,0.00006510308],"about_ca_topic_score_codex":0.0022350429,"about_ca_topic_score_gemma":0.005184858,"teacher_disagreement_score":0.0022350429,"about_ca_system_score_codex":0.000286315,"about_ca_system_score_gemma":0.0003301867,"threshold_uncertainty_score":0.006918013},"labels":[],"label_agreement":null},{"id":"W2003792386","doi":"10.1088/0004-637x/748/1/20","title":"DARK MATTER SUB-HALO COUNTS VIA STAR STREAM CROSSINGS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Halo; Physics; Astrophysics; Dark matter halo; Milky Way; Dark matter; Galactic halo; Galaxy; Astronomy","score_opus":0.006023616620560231,"score_gpt":0.2108009248732029,"score_spread":0.20477730825264268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003792386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947003,0.00007955149,0.0032306076,0.000021523183,0.0000030092879,0.000009400819,0.00043446218,0.00012958965,0.0013914522],"genre_scores_gemma":[0.9976035,0.00003600566,0.0015602715,0.0000036330662,0.000002154648,0.0000051056168,0.0004844391,0.000018112449,0.00028683295],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998202,0.000042754487,0.000009025245,0.000047589852,0.000040211802,0.000040259],"domain_scores_gemma":[0.998733,0.00051663106,0.00027501571,0.00013771317,0.000136527,0.00020105887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072361215,0.00031499483,0.00025380068,0.0008520083,0.00019750754,0.0007397865,0.0003839563,0.00025404495,0.0017450633],"category_scores_gemma":[0.003537098,0.000163795,0.0003999395,0.00073400815,0.0002792844,0.000777997,0.0006291979,0.0002284945,0.0001914209],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045011274,0.00008263573,0.5579578,0.00007309351,0.00017976329,0.00027805186,0.00029849165,0.4091234,0.0042375494,0.010066099,0.0007934252,0.016459566],"study_design_scores_gemma":[0.000031573603,0.00012871229,0.16273722,0.000022822956,0.00006264578,0.00022632835,0.0001419051,0.82226276,0.00680455,0.0061097792,0.0014383845,0.000033364147],"about_ca_topic_score_codex":0.0037763908,"about_ca_topic_score_gemma":0.0033155254,"teacher_disagreement_score":0.0037763908,"about_ca_system_score_codex":0.0005742462,"about_ca_system_score_gemma":0.0002465608,"threshold_uncertainty_score":0.0075088143},"labels":[],"label_agreement":null},{"id":"W2003801041","doi":"10.1088/0004-637x/692/1/584","title":"THE DISCOVERY OF A VERY FAINT X-RAY TRANSIENT IN THE GLOBULAR CLUSTER M15","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"ROSAT; Globular cluster; Luminosity; Neutron star; Galaxy; Transient (computer programming); Star cluster; Extinction (optical mineralogy)","score_opus":0.008550741124573158,"score_gpt":0.22468111340286748,"score_spread":0.21613037227829432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003801041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995086,0.00007363541,0.00010698767,0.000017947872,0.000002674706,0.0000025114723,0.000028495117,0.0000081928765,0.00025101652],"genre_scores_gemma":[0.99922156,0.00004085701,0.00044810594,0.000026183945,0.000004255668,0.0000021509247,0.00010850304,0.0000024115968,0.00014589058],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999367,0.000003619408,0.0000056489544,0.000021802483,0.000012620164,0.000019599],"domain_scores_gemma":[0.999726,0.000023412813,0.00008383812,0.000033643722,0.000028539529,0.00010461071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017976624,0.00014123415,0.0001780138,0.00032229818,0.00045923432,0.0005103883,0.00041784003,0.00044097667,0.00043642736],"category_scores_gemma":[0.0003419617,0.00012288133,0.00019046254,0.00034084663,0.00036151303,0.00029437224,0.0006465147,0.0002170062,0.0001223889],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051887834,0.000080456775,0.7528721,0.000105149906,0.00008110807,0.0030570163,0.0014225397,0.00045271812,0.22634283,0.0012814791,0.00036164108,0.013424159],"study_design_scores_gemma":[0.000014640321,0.00020115505,0.9852667,0.000018643308,0.000040513994,0.0014292699,0.00029105778,0.0008537259,0.0099257175,0.00020677286,0.0017399921,0.00001186176],"about_ca_topic_score_codex":0.002693508,"about_ca_topic_score_gemma":0.004434454,"teacher_disagreement_score":0.002693508,"about_ca_system_score_codex":0.00040847005,"about_ca_system_score_gemma":0.00023080803,"threshold_uncertainty_score":0.0053557158},"labels":[],"label_agreement":null},{"id":"W2003856002","doi":"10.1088/0004-637x/798/2/75","title":"KINEMATICS IN PARTIALLY IONIZED MOLECULAR CLOUDS: IMPLICATIONS FOR THE TRANSITION TO COHERENCE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ionization; Supersonic speed; Photoionization; Physics; Coherence (philosophical gambling strategy); Spectral line; Substructure; Atomic physics; Kinematics; Astrophysics; Mechanics; Ion; Classical mechanics","score_opus":0.013220642292180361,"score_gpt":0.2652947759852162,"score_spread":0.2520741336930359,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003856002","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967667,0.00007994752,0.002256325,0.00013222767,0.0000029371568,0.0000062700824,0.000067831876,0.00003153495,0.0006561622],"genre_scores_gemma":[0.9996358,0.000022087954,0.0002604431,0.0000067666565,0.000001374014,0.0000011735384,0.000029356765,0.000007180784,0.00003570734],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999356,0.000012737945,0.000004477909,0.000015200147,0.000011461589,0.000020489117],"domain_scores_gemma":[0.99955803,0.00012995876,0.00012518506,0.00006198901,0.000043487744,0.00008131216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002161614,0.0002481558,0.00019013701,0.00034763882,0.00040635746,0.0011460208,0.0003922061,0.00035668607,0.00085320463],"category_scores_gemma":[0.0017628798,0.00023748692,0.00031643722,0.0003556179,0.0006338877,0.0008365996,0.0006227268,0.0004484346,0.00006981782],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041167488,0.0001817456,0.514619,0.00007606938,0.00019070294,0.0006071458,0.0015013845,0.3988367,0.059326306,0.013486799,0.0005205135,0.01024187],"study_design_scores_gemma":[0.00010080099,0.0002509949,0.48219988,0.000028696024,0.0000540315,0.00018585564,0.0007069179,0.49965978,0.0068248115,0.008890597,0.0010404882,0.000057207213],"about_ca_topic_score_codex":0.01282678,"about_ca_topic_score_gemma":0.0075306436,"teacher_disagreement_score":0.01282678,"about_ca_system_score_codex":0.00063576153,"about_ca_system_score_gemma":0.00038869088,"threshold_uncertainty_score":0.025504231},"labels":[],"label_agreement":null},{"id":"W2003917323","doi":"10.1088/0004-637x/792/1/37","title":"BANYAN. IV. FUNDAMENTAL PARAMETERS OF LOW-MASS STAR CANDIDATES IN NEARBY YOUNG STELLAR KINEMATIC GROUPS—ISOCHRONAL AGE DETERMINATION USING MAGNETIC EVOLUTIONARY MODELS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":139,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université du Québec à Montréal; Université de Montréal","funders":"","keywords":"Stars; Physics; Astrophysics; Parallax; Metallicity; Proper motion; Magnetic field; Astronomy","score_opus":0.011868996215835122,"score_gpt":0.22051924768872783,"score_spread":0.2086502514728927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2003917323","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9471554,0.00055884453,0.03692409,0.00006605232,0.00001549866,0.000040038045,0.002006283,0.00045963182,0.01277414],"genre_scores_gemma":[0.9748291,0.00013349515,0.018937074,0.0000133952135,0.000007853424,0.00004023655,0.0039068516,0.00007104066,0.0020608865],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999814,0.000036493155,0.000009367025,0.00008759113,0.00003510714,0.000017352366],"domain_scores_gemma":[0.99958354,0.00008047427,0.00014801623,0.00007287195,0.00007639916,0.00003875718],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008771318,0.00025468107,0.00024101992,0.0016961908,0.0005495389,0.0010217077,0.0005435274,0.00023182717,0.0019942855],"category_scores_gemma":[0.0012155715,0.00023840164,0.00036075045,0.0006912892,0.00020241237,0.00046091687,0.00054419145,0.00030504254,0.0009871385],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003038097,0.00006770053,0.8931761,0.00008542323,0.00007641152,0.00010612838,0.00077578897,0.016534045,0.014293304,0.005032267,0.0018041144,0.06774497],"study_design_scores_gemma":[0.000031243017,0.000083817984,0.84921753,0.000043624175,0.000051818675,0.00041731398,0.00024487343,0.120465435,0.011550088,0.0048427274,0.01300948,0.000042038828],"about_ca_topic_score_codex":0.00945355,"about_ca_topic_score_gemma":0.01210583,"teacher_disagreement_score":0.00945355,"about_ca_system_score_codex":0.0007615939,"about_ca_system_score_gemma":0.0003438609,"threshold_uncertainty_score":0.01879704},"labels":[],"label_agreement":null},{"id":"W2004264865","doi":"10.1088/0004-637x/763/1/62","title":"ORIGIN AND GROWTH OF NUCLEAR STAR CLUSTERS AROUND MASSIVE BLACK HOLES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":157,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Globular cluster; Star cluster; Galaxy; Bulge; Stellar population; Velocity dispersion; Stellar mass; Stellar collision; Milky Way; Star formation","score_opus":0.006834074302911793,"score_gpt":0.19884633617561068,"score_spread":0.19201226187269888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004264865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986539,0.000101257276,0.0006682834,0.00001769852,0.0000029287164,0.0000025226727,0.0000126906225,0.000011505317,0.00052914093],"genre_scores_gemma":[0.99949706,0.00003137785,0.00029692025,0.00000272495,0.0000018438903,9.479828e-7,0.000019346217,0.000003001244,0.00014691583],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994934,0.000007633684,0.0000022406416,0.00001803779,0.0000090492695,0.000013621353],"domain_scores_gemma":[0.99978787,0.000025174755,0.00008637609,0.000024205017,0.000022878961,0.000053534583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014981083,0.00014783691,0.00017323051,0.00030310196,0.0004794021,0.00053861644,0.0004320176,0.00025468034,0.0006705722],"category_scores_gemma":[0.0006449162,0.00020669171,0.00024143643,0.00015083182,0.0006075563,0.0003225152,0.0004993501,0.00017082717,0.00016981913],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034949178,0.00009579336,0.797855,0.00011408282,0.0001185569,0.0015487286,0.001722117,0.056063116,0.09581155,0.03211722,0.0005787109,0.013625589],"study_design_scores_gemma":[0.000099002296,0.00042417087,0.778581,0.00005275804,0.00010703088,0.0023052194,0.001072232,0.17668109,0.021575937,0.013462881,0.0055775647,0.000061079176],"about_ca_topic_score_codex":0.0035925424,"about_ca_topic_score_gemma":0.0022307574,"teacher_disagreement_score":0.0035925424,"about_ca_system_score_codex":0.00064259244,"about_ca_system_score_gemma":0.00021681532,"threshold_uncertainty_score":0.007143259},"labels":[],"label_agreement":null},{"id":"W2004274663","doi":"10.1086/522667","title":"Discovery of an Isolated Compact Object at High Galactic Latitude","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Millisecond pulsar; Astrophysics; Pulsar; ROSAT; Astronomy; Neutron star; Pulsar planet; Compact star; Halo; X-ray pulsar; Flux (metallurgy); Observatory; Sky; Millisecond; Galactic halo; Binary pulsar; Galaxy","score_opus":0.014913731889172858,"score_gpt":0.23500408239459827,"score_spread":0.22009035050542541,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004274663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960842,0.00088754133,0.00042673916,0.0000517266,0.000020863747,0.000008158642,0.00010547627,0.00003029217,0.0023849453],"genre_scores_gemma":[0.9984843,0.00020357948,0.0005089523,0.000050245537,0.00003635017,0.0000031032273,0.00031572106,0.0000039389893,0.00039382983],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998869,0.0000048706725,0.000007234063,0.00004284339,0.00003111087,0.000027007794],"domain_scores_gemma":[0.9996706,0.000031017826,0.00010829537,0.000045243833,0.000028670662,0.00011604766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001452757,0.00024593112,0.00032991925,0.0007512913,0.00054315897,0.0012934481,0.00054317625,0.0005386642,0.00095576013],"category_scores_gemma":[0.00028624674,0.00016657096,0.00016106438,0.00048504348,0.00042985132,0.00031707864,0.0007293879,0.00033624537,0.00055390305],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050558,0.00023385107,0.60268706,0.0002387371,0.0001882051,0.028463895,0.0012815864,0.00022659753,0.30687314,0.0024689494,0.0019383422,0.054894082],"study_design_scores_gemma":[0.0000578465,0.0006756618,0.8846816,0.000050211296,0.00021021874,0.05477458,0.0007039442,0.0007350319,0.036401063,0.0007436622,0.020920847,0.000045337212],"about_ca_topic_score_codex":0.00074291945,"about_ca_topic_score_gemma":0.0009153089,"teacher_disagreement_score":0.0012934481,"about_ca_system_score_codex":0.0002192185,"about_ca_system_score_gemma":0.00011007131,"threshold_uncertainty_score":0.0031973124},"labels":[],"label_agreement":null},{"id":"W2004287403","doi":"10.1088/0004-637x/713/1/318","title":"<i>RXTE</i>-BASED 35 DAY CYCLE TURN-ON TIMES FOR HERCULES X-1","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Sky; Astrophysics; Astronomy; Turn (biochemistry); Phase (matter)","score_opus":0.008922100326053164,"score_gpt":0.23685313608534195,"score_spread":0.22793103575928877,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004287403","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95192814,0.00092365843,0.0036601562,0.00012736162,0.000074953474,0.00006602458,0.031706657,0.00093102973,0.010581952],"genre_scores_gemma":[0.9004903,0.00048834924,0.011295506,0.0000747331,0.00012246944,0.00009465628,0.08422462,0.0004482537,0.002761204],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997725,0.000024338156,0.000023501776,0.00006613495,0.00007273755,0.00004089076],"domain_scores_gemma":[0.99879396,0.000139006,0.0006008179,0.00016913265,0.00018480982,0.000112332964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005148383,0.00028922758,0.00021543281,0.0038396502,0.00024799164,0.00063865376,0.00024938514,0.00014744948,0.0023611495],"category_scores_gemma":[0.0015486475,0.000097683536,0.00036856346,0.0021189123,0.000102479506,0.00024359165,0.00045645385,0.00025124234,0.0008607941],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045560236,0.00007743256,0.8736469,0.00021560323,0.000230866,0.00036054602,0.00036550645,0.0067839148,0.026315397,0.001292612,0.020873541,0.06938207],"study_design_scores_gemma":[0.000010803715,0.00003667216,0.9756162,0.000014634876,0.000033998396,0.00019744989,0.000049999053,0.0033824875,0.0042347237,0.00018463598,0.0162201,0.000018157638],"about_ca_topic_score_codex":0.0072589284,"about_ca_topic_score_gemma":0.011411742,"teacher_disagreement_score":0.0072589284,"about_ca_system_score_codex":0.00038602127,"about_ca_system_score_gemma":0.00029965662,"threshold_uncertainty_score":0.014433324},"labels":[],"label_agreement":null},{"id":"W2004309214","doi":"10.1086/593350","title":"The <i>s</i> -Process in Massive Stars at Low Metallicity: The Effect of Primary <sup>14</sup> N from Fast Rotating Stars","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":201,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Nucleosynthesis; Metallicity; Physics; s-process; Astrophysics; r-process; Stars; Neutron star; Nuclear reaction; Stellar nucleosynthesis; Rotation (mathematics); Neutron poison; Halo; Stellar evolution; Neutron; Nuclear physics; Galaxy; Neutron temperature","score_opus":0.008900702939543969,"score_gpt":0.24557869152763923,"score_spread":0.23667798858809524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004309214","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979747,0.00026033953,0.0005156702,0.000018692857,0.000002505978,0.000003582302,0.00007163334,0.000019970741,0.0011328837],"genre_scores_gemma":[0.9992606,0.000108700435,0.00022552896,0.0000070041833,0.0000034174293,0.00000227285,0.00011274754,0.000013065311,0.00026656705],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999124,0.000018735582,0.0000071907143,0.000022826407,0.000018212968,0.000020672724],"domain_scores_gemma":[0.9997625,0.00008023385,0.00005701762,0.000028905955,0.00002841518,0.000043070486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020767529,0.00066286797,0.0003247927,0.00020469945,0.00023219017,0.0004404024,0.00028501643,0.00029611317,0.001478537],"category_scores_gemma":[0.0004897787,0.00012836131,0.0004547247,0.00017287608,0.00026973672,0.00019716828,0.0003977258,0.00014679211,0.0004941473],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002224175,0.00013338859,0.20408207,0.00043373654,0.0002499528,0.0016960884,0.0002307031,0.10910313,0.66104364,0.0018211823,0.00023935645,0.018742504],"study_design_scores_gemma":[0.000159052,0.0016902435,0.4560221,0.000044151013,0.00030972614,0.0010381815,0.0002685658,0.14800619,0.38655883,0.002555922,0.0032994975,0.000047543537],"about_ca_topic_score_codex":0.0013799426,"about_ca_topic_score_gemma":0.0012492589,"teacher_disagreement_score":0.001478537,"about_ca_system_score_codex":0.00031855423,"about_ca_system_score_gemma":0.00011281739,"threshold_uncertainty_score":0.0049461722},"labels":[],"label_agreement":null},{"id":"W2004311486","doi":"10.1086/340973","title":"A Deep Search for Pulsations from the Nearby Isolated Neutron Star RX J1856.5−3754","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Neutron star; Gravitational wave; Stars; Limit (mathematics); Neutron; Gravitation","score_opus":0.02285290540068087,"score_gpt":0.3059616006424043,"score_spread":0.28310869524172344,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004311486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985501,0.00008435483,0.0004567256,0.000024188012,0.0000029100686,0.0000066307452,0.00014691135,0.000020893967,0.00070734223],"genre_scores_gemma":[0.99758947,0.00004113761,0.0012456964,0.000029497345,0.000008560117,0.0000044348526,0.00057062303,0.000006604118,0.00050403504],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999861,0.000010293312,0.000005217282,0.000037427475,0.000037195154,0.000048796148],"domain_scores_gemma":[0.9996964,0.000035446446,0.000083604566,0.000029519246,0.000020864378,0.00013422906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002748611,0.00032334152,0.00039981844,0.0005517764,0.0005022601,0.00037446473,0.00034570112,0.00024799048,0.0013082058],"category_scores_gemma":[0.00040956086,0.00021282648,0.0002638977,0.00031980764,0.00021447263,0.00019176508,0.00080741855,0.0002937913,0.00024187076],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018023956,0.00036068368,0.41741604,0.00019458466,0.00036986475,0.0028988714,0.0010442185,0.002479313,0.5149588,0.0011817929,0.0011052815,0.05618822],"study_design_scores_gemma":[0.00014958136,0.0010212322,0.94974416,0.000017454,0.0002171818,0.0018218058,0.00037164995,0.0044613993,0.037188794,0.0006687591,0.0042950665,0.0000428927],"about_ca_topic_score_codex":0.0016268363,"about_ca_topic_score_gemma":0.0046295794,"teacher_disagreement_score":0.0016268363,"about_ca_system_score_codex":0.0002874394,"about_ca_system_score_gemma":0.00029697918,"threshold_uncertainty_score":0.004376352},"labels":[],"label_agreement":null},{"id":"W2004320363","doi":"10.1088/0004-637x/782/2/100","title":"THE ABSOLUTE MAGNITUDE DISTRIBUTION OF KUIPER BELT OBJECTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":236,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Absolute magnitude; Magnitude (astronomy); Ecliptic; Albedo (alchemy); Population; Mass distribution; Nice model; Planetesimal; Trojan","score_opus":0.004294858928270622,"score_gpt":0.19750647120624715,"score_spread":0.19321161227797654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004320363","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99234164,0.00029251887,0.0005194502,0.00003374083,0.0000054397374,0.0000055195596,0.0011744556,0.0000789226,0.0055482783],"genre_scores_gemma":[0.9966235,0.000128988,0.00034282837,0.000016754591,0.000021796848,0.0000053943936,0.0019705666,0.000013697175,0.00087661546],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982005,0.00001772179,0.000012077007,0.000065016786,0.000053534673,0.000031640993],"domain_scores_gemma":[0.9989396,0.00013856974,0.00049971836,0.000085788946,0.00018969341,0.00014675241],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021371814,0.00017182285,0.00012906877,0.0014452436,0.00021797609,0.0007357383,0.0002521526,0.00015182297,0.0027482938],"category_scores_gemma":[0.0013645861,0.00010530589,0.00010694598,0.0008186342,0.00023392339,0.0006074981,0.00036921777,0.00017739685,0.0010079022],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000084339954,0.000011982935,0.9777414,0.000029487928,0.000032595213,0.0000482365,0.00028788927,0.0002811549,0.0044672373,0.0002946624,0.0006249561,0.016096018],"study_design_scores_gemma":[0.0000010557417,0.000013563332,0.9988256,0.0000029182536,0.000004132919,0.00008893926,0.00006997853,0.000102840204,0.00024233399,0.000058936377,0.00058720075,0.000002338431],"about_ca_topic_score_codex":0.0013025674,"about_ca_topic_score_gemma":0.0017307684,"teacher_disagreement_score":0.0027482938,"about_ca_system_score_codex":0.00016394611,"about_ca_system_score_gemma":0.00005829438,"threshold_uncertainty_score":0.009193897},"labels":[],"label_agreement":null},{"id":"W2004476873","doi":"10.1088/0004-637x/725/2/1877","title":"LBT/LUCIFER OBSERVATIONS OF THE<i>z</i>∼ 2 LENSED GALAXY J0900+2234","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Metallicity; Photometry (optics); Astronomy; Type-cD galaxy; Galaxy formation and evolution; Stars","score_opus":0.011451216679972086,"score_gpt":0.2090451569389172,"score_spread":0.1975939402589451,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004476873","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99174786,0.00010084997,0.00045128603,0.000048062175,0.0000055068435,0.000016375725,0.0024305342,0.0003353059,0.0048641427],"genre_scores_gemma":[0.9899963,0.00012509878,0.002187632,0.00008530947,0.000024790697,0.00003182512,0.005857668,0.000062805615,0.0016285481],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998165,0.000012798233,0.000005860648,0.000043237353,0.00005013306,0.000071543516],"domain_scores_gemma":[0.9997651,0.000014039551,0.00007098751,0.000023220913,0.000032904478,0.00009371442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019197473,0.00031328233,0.00034955007,0.0012713827,0.00050436,0.00042672173,0.00064172124,0.00023628917,0.0015812425],"category_scores_gemma":[0.00024000402,0.0002364679,0.0002313628,0.0008085962,0.0002062995,0.00022064908,0.00058635167,0.00030114473,0.00056083745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015298988,0.0006035355,0.5801376,0.00018324335,0.00029575996,0.0018123032,0.00048364024,0.004317221,0.36449778,0.0008315445,0.011366132,0.033941343],"study_design_scores_gemma":[0.000060234786,0.00014987486,0.9849904,0.00001139811,0.000051539537,0.00029472183,0.00005713847,0.003570831,0.0067734974,0.000091089925,0.00393025,0.0000189477],"about_ca_topic_score_codex":0.019904345,"about_ca_topic_score_gemma":0.037930585,"teacher_disagreement_score":0.019904345,"about_ca_system_score_codex":0.0009084819,"about_ca_system_score_gemma":0.0002824711,"threshold_uncertainty_score":0.039577007},"labels":[],"label_agreement":null},{"id":"W2004523188","doi":"10.1088/0004-637x/702/2/1662","title":"PLANETARY MIGRATION AND ECCENTRICITY AND INCLINATION RESONANCES IN EXTRASOLAR PLANETARY SYSTEMS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph","funders":"","keywords":"Eccentricity (behavior); Physics; Planet; Resonance (particle physics); Astrophysics; Planetary migration; Orbital eccentricity; Planetary mass; Exoplanet; Mean motion; Planetary system; Atomic physics","score_opus":0.00832831146878027,"score_gpt":0.21217815517692862,"score_spread":0.20384984370814835,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004523188","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984804,0.000111681125,0.00024348358,0.000027143406,0.0000026581329,0.0000015168467,0.000010987321,0.000006285147,0.0011158346],"genre_scores_gemma":[0.9996568,0.00003769915,0.00013558698,0.000003445329,0.0000025285967,0.0000010734868,0.000017624552,0.0000022916786,0.0001429122],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998652,0.00003974341,0.000016072818,0.000031772895,0.000023353585,0.000023869581],"domain_scores_gemma":[0.9990615,0.0003211453,0.00033195314,0.00010409281,0.00006404665,0.00011727066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024714897,0.00015557402,0.00015983556,0.00054138375,0.0005022113,0.00047844794,0.00015819694,0.00042761312,0.0009272789],"category_scores_gemma":[0.0030026636,0.0001633195,0.00014766095,0.00035108931,0.00060058245,0.0005567375,0.0007343843,0.0002210812,0.00017451106],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007016609,0.00008236111,0.8643918,0.00012285552,0.000089586916,0.0011173063,0.0030861967,0.03646416,0.052356433,0.007533016,0.000492911,0.033561707],"study_design_scores_gemma":[0.000022287066,0.00014505285,0.9715376,0.000015145531,0.000019584153,0.0009740725,0.00070308807,0.019217692,0.001850996,0.0040113907,0.001480739,0.000022378501],"about_ca_topic_score_codex":0.001695582,"about_ca_topic_score_gemma":0.0021892034,"teacher_disagreement_score":0.001695582,"about_ca_system_score_codex":0.00028733746,"about_ca_system_score_gemma":0.00011823096,"threshold_uncertainty_score":0.0033714175},"labels":[],"label_agreement":null},{"id":"W2004559889","doi":"10.1088/0004-637x/693/2/1392","title":"THE INTEGRATED POLARIZATION OF SPIRAL GALAXY DISKS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Faraday effect; Polarization (electrochemistry); Spiral galaxy; Radio galaxy; Magnetic field; Galaxy; Redshift","score_opus":0.007518224730869295,"score_gpt":0.2246295388543064,"score_spread":0.2171113141234371,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004559889","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926495,0.00019719306,0.00451546,0.000047976762,0.0000045704687,0.0000035827252,0.00039864873,0.0001162565,0.002066667],"genre_scores_gemma":[0.999065,0.000052910556,0.0004308128,0.0000036360334,0.000002799673,0.0000028032907,0.0002136177,0.000010341731,0.00021812301],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999207,0.000013908753,0.0000026302096,0.000023032675,0.000013084818,0.000026540929],"domain_scores_gemma":[0.9995185,0.00016799664,0.0000900987,0.00005600681,0.00010018296,0.00006724234],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019460966,0.00046180436,0.00022822362,0.00067884783,0.00021936695,0.0006623315,0.00036262983,0.00024144033,0.0017126112],"category_scores_gemma":[0.0013210211,0.0001888059,0.0003805669,0.00057885924,0.00025649677,0.0004850028,0.00024130825,0.00020006095,0.00026756647],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005656955,0.00007343933,0.22702532,0.00007392862,0.00016964847,0.0003382669,0.00018703648,0.7245608,0.023980977,0.005327406,0.00092717935,0.016770279],"study_design_scores_gemma":[0.00007835409,0.00015486128,0.10994785,0.000020955798,0.00010511848,0.00040258048,0.00008365892,0.87257075,0.005864993,0.009377364,0.0013447738,0.000048762085],"about_ca_topic_score_codex":0.0039426587,"about_ca_topic_score_gemma":0.0022456024,"teacher_disagreement_score":0.0039426587,"about_ca_system_score_codex":0.0005835899,"about_ca_system_score_gemma":0.00013132676,"threshold_uncertainty_score":0.007839441},"labels":[],"label_agreement":null},{"id":"W2004629459","doi":"10.1086/509146","title":"Discovery of the Brightest T Dwarf in the Northern Hemisphere","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Proper motion; Photometry (optics); Physics; Astrophysics; Sky; Astronomy; Stellar classification; Circumbinary planet; Infrared; Stars","score_opus":0.0056029324984847575,"score_gpt":0.1955544938079184,"score_spread":0.18995156130943364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004629459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950654,0.00035940524,0.00017249829,0.00010148924,0.000012735315,0.000004926341,0.00025010091,0.00005311885,0.0039803805],"genre_scores_gemma":[0.9976949,0.00016587944,0.00044851904,0.00007134419,0.000028195562,0.000002748436,0.00052585895,0.000011506323,0.0010510612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986565,0.000008736461,0.00000558332,0.00003468841,0.000043091815,0.000042176493],"domain_scores_gemma":[0.99975175,0.000016110893,0.00007266546,0.000019067385,0.00002855205,0.000111771194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026253477,0.00014190207,0.00025915922,0.00082963787,0.00062611274,0.00095067703,0.00023374481,0.0003039739,0.0012249302],"category_scores_gemma":[0.00034475263,0.000103027625,0.00012854161,0.0005398659,0.000402411,0.00021199165,0.0006105531,0.00019278716,0.0005728815],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008169248,0.00010251326,0.6999131,0.00014684473,0.00005832775,0.010328144,0.0028109404,0.00030378587,0.19918059,0.0016777833,0.0058820974,0.07877895],"study_design_scores_gemma":[0.0000328542,0.00016596442,0.9658157,0.000018743644,0.000030845127,0.0050423043,0.00048128847,0.00041160584,0.009362443,0.0005304253,0.01809048,0.000017315459],"about_ca_topic_score_codex":0.008577344,"about_ca_topic_score_gemma":0.0118294805,"teacher_disagreement_score":0.008577344,"about_ca_system_score_codex":0.00047377395,"about_ca_system_score_gemma":0.00038385525,"threshold_uncertainty_score":0.017054856},"labels":[],"label_agreement":null},{"id":"W2004633439","doi":"10.1088/0004-637x/774/2/99","title":"A HIGH-RESOLUTION SPECTROSCOPIC SEARCH FOR THE REMAINING DONOR FOR TYCHO'S SUPERNOVA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Astrometry; Supernova; Hubble space telescope; Stars; Spectroscopy; Telescope; Supernova remnant; Hubble Deep Field South; Near-Earth supernova","score_opus":0.018854249176530766,"score_gpt":0.25828546432261373,"score_spread":0.23943121514608295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004633439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99852055,0.00022307181,0.0005471931,0.000017956994,0.000006403405,0.000015619351,0.00013785416,0.000009579,0.0005217231],"genre_scores_gemma":[0.9973049,0.00012756196,0.0015880173,0.00003332321,0.0000122566435,0.000008976975,0.0006537051,0.0000050629196,0.00026614658],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991786,0.000006941254,0.000009862228,0.000029280316,0.000016853217,0.000019168268],"domain_scores_gemma":[0.99942744,0.00006887875,0.00014707296,0.00006444657,0.00007139438,0.00022082457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043495672,0.0002550886,0.00030737653,0.0013320447,0.0005469848,0.0005534326,0.0003723046,0.00037828737,0.0012168869],"category_scores_gemma":[0.0005420442,0.00010093745,0.00026215782,0.0005934917,0.00021707077,0.00029638462,0.00057714095,0.00024951404,0.00040058757],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013038541,0.00003669383,0.9444256,0.00003663159,0.0000530001,0.0025568146,0.00028843468,0.00008208473,0.0444721,0.00019673794,0.00013120566,0.007590471],"study_design_scores_gemma":[0.000017952241,0.00038495872,0.9716061,0.000024518951,0.00010830832,0.01041144,0.0013032787,0.0007645749,0.011800701,0.00033361916,0.0032293275,0.00001528324],"about_ca_topic_score_codex":0.0015054524,"about_ca_topic_score_gemma":0.0026206956,"teacher_disagreement_score":0.0015054524,"about_ca_system_score_codex":0.00015545644,"about_ca_system_score_gemma":0.00036248102,"threshold_uncertainty_score":0.004070878},"labels":[],"label_agreement":null},{"id":"W2004698958","doi":"10.1086/586734","title":"Beyond Inside-Out Growth: Formation and Evolution of Disk Outskirts","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":386,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Star formation; Spiral galaxy; RADIUS; Stars; Galaxy; Halo; Dark matter halo; Surface brightness; Drop (telecommunication); Stellar mass; Astronomy","score_opus":0.0076920981556483714,"score_gpt":0.1980374564552914,"score_spread":0.19034535829964302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004698958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942577,0.00012520739,0.0019022139,0.00012113338,0.000018130446,0.000016712891,0.00020308633,0.000075417054,0.0032803023],"genre_scores_gemma":[0.99803454,0.00006299544,0.001013188,0.000030325355,0.000006410355,0.000009146219,0.00018687194,0.000034311885,0.0006221392],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998398,0.00003013249,0.0000066249395,0.000031142947,0.00002351053,0.00006874976],"domain_scores_gemma":[0.9992982,0.00017514192,0.00010705822,0.00008455703,0.000071563605,0.0002634166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030720924,0.0006156115,0.00082169863,0.00038998344,0.001085405,0.0015749264,0.0012464259,0.0012997171,0.002141826],"category_scores_gemma":[0.0023865052,0.0004954658,0.0006141991,0.00033477385,0.0012758183,0.0010131202,0.0010266443,0.0009170623,0.00021205714],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020272666,0.0001574107,0.018681778,0.000043874254,0.00005115868,0.0007642708,0.00025219994,0.9681382,0.005964975,0.003540088,0.0003633377,0.00183997],"study_design_scores_gemma":[0.00007570696,0.000090256195,0.005879175,0.000010931249,0.000020174557,0.000108582644,0.00013429487,0.990067,0.0015821811,0.0014439279,0.00056222477,0.000025496076],"about_ca_topic_score_codex":0.026724106,"about_ca_topic_score_gemma":0.011272189,"teacher_disagreement_score":0.026724106,"about_ca_system_score_codex":0.0012472882,"about_ca_system_score_gemma":0.0009522376,"threshold_uncertainty_score":0.053137124},"labels":[],"label_agreement":null},{"id":"W2004699585","doi":"10.1086/340663","title":"The Cluster<i>M</i><sub>gas</sub>‐<i>T</i><sub>X</sub>Relation: Evidence for a High Level of Preheating","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Cluster (spacecraft); Virial theorem; Physics; RADIUS; Intracluster medium; Entropy (arrow of time); Mass fraction; Astrophysics; Thermodynamics; Mechanics; Statistical physics; Galaxy cluster; Galaxy","score_opus":0.056682832405465,"score_gpt":0.2687060185231079,"score_spread":0.21202318611764287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004699585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940521,0.0004739361,0.0016694376,0.000111504174,0.0000046759087,0.0000073100873,0.00006786828,0.0001151136,0.003497975],"genre_scores_gemma":[0.99914825,0.00006175517,0.0005041289,0.000024516392,0.0000068614695,0.000005248813,0.00003950823,0.000012890985,0.00019677161],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998852,0.000007283359,0.0000037091572,0.000055383807,0.000018687891,0.000029675393],"domain_scores_gemma":[0.9992939,0.000187908,0.0003081084,0.00010757337,0.000044762754,0.000057773657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015513496,0.000212591,0.00020494378,0.0005264804,0.00045937859,0.0007038353,0.000564721,0.00051221077,0.0010580578],"category_scores_gemma":[0.0009137444,0.00029141895,0.00017120565,0.00055839313,0.0009870817,0.0004886399,0.0005364295,0.0005806692,0.00024817212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000707673,0.000096487565,0.5397988,0.0002296365,0.00012340829,0.0015091783,0.001686197,0.008205788,0.40252146,0.02629546,0.0017314401,0.017094506],"study_design_scores_gemma":[0.000031223375,0.00014318443,0.89505774,0.000012956443,0.000050235765,0.001114161,0.0002203111,0.020235064,0.07567631,0.0057431837,0.0016844054,0.000031204592],"about_ca_topic_score_codex":0.0013413485,"about_ca_topic_score_gemma":0.0012082101,"teacher_disagreement_score":0.0013413485,"about_ca_system_score_codex":0.00047890743,"about_ca_system_score_gemma":0.00016286928,"threshold_uncertainty_score":0.0035396218},"labels":[],"label_agreement":null},{"id":"W2004853063","doi":"10.1086/339915","title":"Magnetic Fields in Star‐forming Molecular Clouds. IV. Polarimetry of the Filamentary NGC 2068 Cloud in Orion B","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Polarization (electrochemistry); Polarimetry; Sky; Reflection nebula; Magnetic field; Molecular cloud; Nebula; James Clerk Maxwell Telescope; Orion Nebula","score_opus":0.007650372519651547,"score_gpt":0.213761571801369,"score_spread":0.20611119928171745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004853063","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991967,0.00005341524,0.00008098472,0.000013107194,0.0000012383094,0.0000015870515,0.00008751819,0.00000866678,0.00055667706],"genre_scores_gemma":[0.99937904,0.00005343115,0.00025429414,0.0000070634223,0.000006835985,0.0000016365422,0.0001680275,0.0000022696686,0.00012729662],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999664,0.0000033537804,0.0000015039311,0.000008597074,0.000008416766,0.0000116482925],"domain_scores_gemma":[0.99986374,0.000013100729,0.000063644045,0.000007813296,0.000019464374,0.00003225425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006237727,0.00014721304,0.00008856088,0.000574727,0.00027566572,0.000268637,0.00014915757,0.00015206871,0.0005045812],"category_scores_gemma":[0.0002322834,0.00008183601,0.00008311346,0.00035592096,0.00012617007,0.000119914905,0.00023452862,0.00013790609,0.0001388355],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004640073,0.00006581917,0.7597954,0.000053058957,0.00004024992,0.0007563262,0.0005778622,0.0012211499,0.21783409,0.00032830058,0.0004233859,0.018440265],"study_design_scores_gemma":[0.000008063514,0.000034708915,0.99564725,0.0000056214935,0.000009589606,0.00017741103,0.00007417701,0.0007903903,0.0026981896,0.000051235587,0.00050035975,0.000002854812],"about_ca_topic_score_codex":0.0056971083,"about_ca_topic_score_gemma":0.0058866497,"teacher_disagreement_score":0.0056971083,"about_ca_system_score_codex":0.00021963735,"about_ca_system_score_gemma":0.00006301148,"threshold_uncertainty_score":0.011327863},"labels":[],"label_agreement":null},{"id":"W2004911908","doi":"10.1086/309172","title":"A New Probe of the Molecular Gas in Galaxies: Application to M101","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Extinction (optical mineralogy); Galaxy; Spiral galaxy; Flux (metallurgy); Spiral (railway); Interstellar medium; Metallicity; Hydrogen molecule; Photodissociation","score_opus":0.003657601242865633,"score_gpt":0.19961825891772242,"score_spread":0.1959606576748568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004911908","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86021185,0.0063923374,0.11748494,0.0009368055,0.00008089908,0.00011370583,0.0007032929,0.0013649189,0.012711153],"genre_scores_gemma":[0.9223225,0.0013559841,0.07378055,0.00027775756,0.00008845879,0.00010764156,0.0002931987,0.000039518458,0.0017343928],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999923,0.000013790678,0.000002422749,0.000028821294,0.000018778033,0.000013200585],"domain_scores_gemma":[0.99984074,0.000048300135,0.00002520708,0.00003251441,0.000014710621,0.000038656253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001892917,0.00020578028,0.00019183238,0.0007774375,0.0002811264,0.0004972554,0.00048842013,0.0006508817,0.0011360034],"category_scores_gemma":[0.00039043746,0.00016611163,0.00018094922,0.00061798794,0.00036074012,0.00038131716,0.00070942397,0.00026331138,0.00033452502],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020474367,0.00014881633,0.081474856,0.0002095283,0.000060355997,0.00048218877,0.00032910059,0.005285868,0.7489089,0.0065526194,0.0012229752,0.15512003],"study_design_scores_gemma":[0.00018695416,0.0011166113,0.5902601,0.00012104824,0.00015923621,0.004504867,0.00079900067,0.15202685,0.19207135,0.012931529,0.04566798,0.00015457107],"about_ca_topic_score_codex":0.001532644,"about_ca_topic_score_gemma":0.0017047735,"teacher_disagreement_score":0.001532644,"about_ca_system_score_codex":0.00038294424,"about_ca_system_score_gemma":0.00013104118,"threshold_uncertainty_score":0.0038003325},"labels":[],"label_agreement":null},{"id":"W2004915072","doi":"10.1088/0004-637x/769/1/7","title":"THE AGE AND STELLAR PARAMETERS OF THE PROCYON BINARY SYSTEM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Luminosity; RADIUS; Stellar evolution; Helium; Hertzsprung–Russell diagram; Stars; Astrometry; Solar mass; Binary star","score_opus":0.008827352168689883,"score_gpt":0.19732889182191027,"score_spread":0.1885015396532204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004915072","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99450994,0.00027553967,0.00038495797,0.000012855737,0.000003838821,0.0000058519518,0.00037907704,0.000021178452,0.004406669],"genre_scores_gemma":[0.997593,0.00013115199,0.00056359346,0.000005938801,0.0000033301108,0.0000052712094,0.00084755523,0.000010319375,0.0008398034],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994195,0.0000067572482,0.0000045888,0.000019986364,0.000012417771,0.000014351911],"domain_scores_gemma":[0.9998374,0.000030098186,0.00004752699,0.000022495555,0.000029123348,0.000033383974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011897127,0.00016043945,0.00015643843,0.0005906727,0.00033201597,0.00044523325,0.00012671312,0.00015135176,0.0019198714],"category_scores_gemma":[0.00047293352,0.00009338526,0.00009165826,0.0003028963,0.00015035651,0.000261517,0.00038580236,0.00029089156,0.00070626894],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005284765,0.00005321515,0.9227328,0.000060461673,0.000042635867,0.0004544769,0.00043485887,0.006063927,0.020851789,0.0024849083,0.0013148964,0.044977497],"study_design_scores_gemma":[0.000027304772,0.00021839203,0.9720747,0.000024515037,0.00003201785,0.0016891317,0.00035965268,0.007728509,0.0072180214,0.00096875074,0.0096405,0.000018385936],"about_ca_topic_score_codex":0.0021647648,"about_ca_topic_score_gemma":0.0019941232,"teacher_disagreement_score":0.0021647648,"about_ca_system_score_codex":0.00021989214,"about_ca_system_score_gemma":0.00012558683,"threshold_uncertainty_score":0.0064225793},"labels":[],"label_agreement":null},{"id":"W2004963488","doi":"10.1086/504844","title":"Evidence for Shocked Molecular Gas in the Galactic Supernova Remnant CTB 109 (G109.1-1.0)","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Molecular cloud; Astrophysics; Supernova remnant; Astronomy; Observatory; Supernova; Galactic Center; Stars","score_opus":0.020776030914638473,"score_gpt":0.25840805761965246,"score_spread":0.237632026705014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2004963488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98878515,0.00094697316,0.0003056094,0.0005260553,0.0003038037,0.000034567176,0.0009334095,0.00012750927,0.008036841],"genre_scores_gemma":[0.9934708,0.00029504165,0.00041624525,0.00029955443,0.00012931287,0.0000118247835,0.001684058,0.00004267008,0.003650498],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998209,0.000017952281,0.000021985505,0.000055001234,0.000050253002,0.000033900047],"domain_scores_gemma":[0.9986665,0.00022640462,0.00034379662,0.00015494988,0.0002538626,0.00035452592],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000405356,0.0002573512,0.00038474004,0.00095504057,0.0006985818,0.0011178406,0.00070973125,0.0017141071,0.009871682],"category_scores_gemma":[0.0012676085,0.00025356218,0.0001977693,0.0006469511,0.00063718064,0.00038708406,0.00073322933,0.00061409606,0.0028555754],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017100319,0.00028954647,0.17544366,0.00096658734,0.00022847873,0.011332464,0.0006476865,0.0002476476,0.7820333,0.0028234397,0.007037195,0.01723992],"study_design_scores_gemma":[0.00037657007,0.0008613316,0.9107829,0.00012520685,0.00021186512,0.00852938,0.0007088892,0.00078798714,0.05255337,0.0012759471,0.023729868,0.00005675747],"about_ca_topic_score_codex":0.001112059,"about_ca_topic_score_gemma":0.0011002388,"teacher_disagreement_score":0.009871682,"about_ca_system_score_codex":0.00022423839,"about_ca_system_score_gemma":0.00016829725,"threshold_uncertainty_score":0.033024073},"labels":[],"label_agreement":null},{"id":"W2005044076","doi":"10.1088/0004-637x/773/1/73","title":"THE SEEDS DIRECT IMAGING SURVEY FOR PLANETS AND SCATTERED DUST EMISSION IN DEBRIS DISK SYSTEMS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Planet; Debris disk; Debris; Stars; Planetary system; Direct imaging; Exoplanet; Giant planet","score_opus":0.011076123184548925,"score_gpt":0.23433681923688257,"score_spread":0.22326069605233365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005044076","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99414057,0.00026207726,0.00060576276,0.00005930602,0.000003929521,0.000029946736,0.001626416,0.000074383075,0.0031976239],"genre_scores_gemma":[0.99373513,0.0001401848,0.0023233395,0.00002796406,0.000008703039,0.000013712083,0.002798938,0.00001361298,0.00093846157],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997893,0.000020186579,0.00001423498,0.00005134785,0.00009039943,0.000034690656],"domain_scores_gemma":[0.99916375,0.000073003524,0.00024781332,0.000078879944,0.00017645209,0.0002600762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030256726,0.00018467993,0.00016248382,0.0020853966,0.00037212294,0.00040194613,0.00022818989,0.00016387686,0.0011121321],"category_scores_gemma":[0.0006590896,0.000163825,0.00015000509,0.00072888174,0.00023347106,0.0003034449,0.00071477355,0.0001270537,0.0004489986],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010720773,0.00007724822,0.9511614,0.000038677834,0.000034156972,0.00040218682,0.000393937,0.0001193794,0.028374812,0.00018641596,0.0019454585,0.017159037],"study_design_scores_gemma":[0.0000069754756,0.00004200989,0.9940116,0.0000059274435,0.00001388454,0.0008181912,0.00014266881,0.00022329601,0.002605701,0.000040012666,0.00208595,0.0000037672094],"about_ca_topic_score_codex":0.008990227,"about_ca_topic_score_gemma":0.02040203,"teacher_disagreement_score":0.008990227,"about_ca_system_score_codex":0.0002856421,"about_ca_system_score_gemma":0.0003096912,"threshold_uncertainty_score":0.01787579},"labels":[],"label_agreement":null},{"id":"W2005059937","doi":"10.1086/500788","title":"Braking the Gas in the β Pictoris Disk","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Radiation; Evaporation; Ionization; Atomic physics; Ion; Nuclear physics; Thermodynamics","score_opus":0.007936053458197749,"score_gpt":0.2287518634110788,"score_spread":0.22081580995288105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005059937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98821825,0.0016252705,0.00090020034,0.00010550893,0.000029253988,0.000010585457,0.000089707864,0.00011564352,0.008905718],"genre_scores_gemma":[0.9986247,0.0002944232,0.00037533138,0.000047657137,0.000010594651,0.000007260413,0.000042556927,0.000008499267,0.00058901124],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999534,0.0000043739055,0.000002462573,0.000017044305,0.000007975618,0.000014718173],"domain_scores_gemma":[0.9999342,0.000017137552,0.000022665146,0.0000065520603,0.0000041952544,0.00001526356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000057557223,0.0002790933,0.00017434108,0.0003293335,0.00041570535,0.00079555134,0.00028346793,0.00027480998,0.002583536],"category_scores_gemma":[0.00025719323,0.00018179386,0.00011729836,0.00023872007,0.00039233378,0.00037101776,0.00042392942,0.00020947286,0.00047292025],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089451397,0.00018652085,0.33289465,0.00053940824,0.00016736308,0.007188911,0.0008671002,0.014945291,0.5694026,0.009577877,0.0026953353,0.06064045],"study_design_scores_gemma":[0.00020653984,0.0012459144,0.8018513,0.00023220835,0.00017179153,0.0064219525,0.0017815507,0.041715287,0.10389474,0.011840673,0.030553162,0.000084926585],"about_ca_topic_score_codex":0.00063318486,"about_ca_topic_score_gemma":0.0005940025,"teacher_disagreement_score":0.002583536,"about_ca_system_score_codex":0.00025833526,"about_ca_system_score_gemma":0.00010013043,"threshold_uncertainty_score":0.008642793},"labels":[],"label_agreement":null},{"id":"W2005075923","doi":"10.1086/321345","title":"The Power Spectrum Dependence of Dark Matter Halo Concentrations","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":487,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Halo; Dark matter; Dark matter halo; Cold dark matter; Redshift; Spectral density; Milky Way; Hot dark matter; Amplitude","score_opus":0.005997918561357841,"score_gpt":0.21888976972751503,"score_spread":0.2128918511661572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005075923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9908922,0.0000965528,0.0037982508,0.00016816205,0.000014350471,0.000010995189,0.00017978225,0.000096261996,0.0047434573],"genre_scores_gemma":[0.99827814,0.000053390362,0.0010992216,0.000029937117,0.000004752794,0.000009696809,0.00016590915,0.00003674372,0.00032226188],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998299,0.000050550076,0.0000066453945,0.000029569681,0.000035310244,0.000047964895],"domain_scores_gemma":[0.9977422,0.0014426648,0.00020463357,0.00023240711,0.00021727651,0.00016090205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006033766,0.000344597,0.00034734383,0.0006738931,0.00036172624,0.0006795997,0.0006636898,0.0005796761,0.0015406037],"category_scores_gemma":[0.0059822747,0.00025934857,0.0006674283,0.00043173356,0.00065678207,0.00079322926,0.00049787154,0.0006997845,0.00017891449],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001113133,0.0000689234,0.019845728,0.00004386448,0.00008314487,0.00022197099,0.00010725118,0.9659759,0.005089058,0.0048935926,0.0006123504,0.0029470543],"study_design_scores_gemma":[0.000012652156,0.00002322815,0.0036390517,0.000004632808,0.000008353438,0.000023469547,0.000017553053,0.9939904,0.0011371721,0.0010322166,0.00010351576,0.000007763127],"about_ca_topic_score_codex":0.007822318,"about_ca_topic_score_gemma":0.0032925508,"teacher_disagreement_score":0.007822318,"about_ca_system_score_codex":0.00056307873,"about_ca_system_score_gemma":0.00033976696,"threshold_uncertainty_score":0.015553534},"labels":[],"label_agreement":null},{"id":"W2005094094","doi":"10.1086/589761","title":"Supernova 1996cr: SN 1987A’s Wild Cousin?","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Physics; Supernova; Astrophysics; Pair-instability supernova; Galaxy; Astronomy; Very-long-baseline interferometry; Line (geometry); Telescope; Ejecta","score_opus":0.015159006981314494,"score_gpt":0.22469857997510626,"score_spread":0.20953957299379175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005094094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95626336,0.008384296,0.00079583755,0.0080356365,0.00075577025,0.00006214516,0.0016672087,0.00014421898,0.023891542],"genre_scores_gemma":[0.97315717,0.0051834807,0.00090702844,0.0020665294,0.0009220921,0.000016644339,0.0030180253,0.0000811067,0.014647908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981886,0.000014496608,0.000013816306,0.00005113567,0.000046164198,0.000055525834],"domain_scores_gemma":[0.9994325,0.000034302582,0.00018653771,0.000075338445,0.00006149355,0.00020980899],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043041757,0.00037462683,0.00034746126,0.0010830672,0.0010319941,0.00096653,0.00038194712,0.0008071228,0.0049657947],"category_scores_gemma":[0.0012351973,0.0001427021,0.0002282876,0.0013744032,0.00043172718,0.00074815983,0.0007908417,0.00094365474,0.0011864337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003850362,0.00025671968,0.81512296,0.00012947537,0.00010604624,0.02500228,0.0023019998,0.00013934293,0.0025606134,0.0072017913,0.035904266,0.110889465],"study_design_scores_gemma":[0.000040497143,0.00031321013,0.68262774,0.00018348798,0.000082527,0.09765771,0.0031955522,0.00069346343,0.0009921017,0.0027800654,0.21138662,0.000047072586],"about_ca_topic_score_codex":0.024230001,"about_ca_topic_score_gemma":0.040936578,"teacher_disagreement_score":0.024230001,"about_ca_system_score_codex":0.00046015234,"about_ca_system_score_gemma":0.00055028236,"threshold_uncertainty_score":0.048177958},"labels":[],"label_agreement":null},{"id":"W2005114148","doi":"10.1086/340560","title":"The MACHO Project Large Magellanic Cloud Variable Star Inventory. XII. Three Cepheid Variables in Eclipsing Binaries","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Cepheid variable; Astrophysics; Physics; Light curve; Large Magellanic Cloud; RADIUS; Radial velocity; Variable star; Astronomy; Orbital period; Eclipse; Stars","score_opus":0.017816923149976658,"score_gpt":0.22495417078898636,"score_spread":0.2071372476390097,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005114148","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.089339934,0.0012446236,0.0023293102,0.00097253703,0.00012387754,0.00027663854,0.874767,0.0035560818,0.027389955],"genre_scores_gemma":[0.10125802,0.0003613702,0.0073345257,0.0001448143,0.000083561645,0.0002707919,0.88241875,0.000390758,0.0077373413],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99951386,0.00004633061,0.000050846043,0.00007023388,0.00022390168,0.00009476834],"domain_scores_gemma":[0.99813074,0.00011548741,0.00040150847,0.00031220462,0.0005630026,0.0004771283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010002648,0.0005126467,0.0006693501,0.004646272,0.0007790163,0.0018230226,0.0011363443,0.00042069072,0.010052967],"category_scores_gemma":[0.002793476,0.00037600021,0.00032772328,0.0045150793,0.000182161,0.0014432982,0.003115774,0.000602786,0.005920853],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013374181,0.00032198319,0.2600718,0.0005488915,0.00021585512,0.00019219921,0.0004368443,0.001202119,0.003314632,0.004801011,0.5700365,0.15752067],"study_design_scores_gemma":[0.00036279316,0.00012561397,0.6137908,0.00015433316,0.0001415151,0.00020660508,0.00046476728,0.004560107,0.0032039518,0.003672918,0.3732661,0.00005049718],"about_ca_topic_score_codex":0.041573584,"about_ca_topic_score_gemma":0.05110966,"teacher_disagreement_score":0.041573584,"about_ca_system_score_codex":0.0007952471,"about_ca_system_score_gemma":0.0015231633,"threshold_uncertainty_score":0.08266318},"labels":[],"label_agreement":null},{"id":"W2005114984","doi":"10.1088/0004-637x/764/1/98","title":"METALLICITY EFFECT ON LOW-MASS X-RAY BINARY FORMATION IN GLOBULAR CLUSTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Metallicity; Galaxy; Luminosity; Elliptical galaxy; Sigma; Virgo Cluster; Star formation","score_opus":0.004818524194605321,"score_gpt":0.2005200599676794,"score_spread":0.1957015357730741,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005114984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991935,0.00007876713,0.000011402523,0.00003053453,0.000002174127,8.9346054e-7,0.00003804029,0.0000016413004,0.0006430855],"genre_scores_gemma":[0.9993198,0.000024888843,0.000008185426,0.000007675721,0.0000016280998,6.0993455e-7,0.00005515915,0.0000016095125,0.000580425],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987006,0.00002670405,0.0000088071365,0.000037109214,0.000017102104,0.000040210092],"domain_scores_gemma":[0.99909604,0.00020835003,0.0002159587,0.0000678365,0.00011622343,0.0002956065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002238951,0.000079820005,0.00014298515,0.00041278396,0.00046593355,0.00077646424,0.00020235234,0.00027251424,0.0039880653],"category_scores_gemma":[0.0014829406,0.00008153705,0.00010813934,0.00029059383,0.00031975855,0.00019660324,0.000544908,0.00016449996,0.0004524202],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060483546,0.00007513057,0.98461807,0.00001644674,0.000030495174,0.00013826205,0.00038900969,0.00035244014,0.0077412007,0.0004522731,0.0003006289,0.005281286],"study_design_scores_gemma":[0.000006479097,0.000032402437,0.9987035,0.0000030243766,0.000011099083,0.000052127853,0.0002551716,0.00018215572,0.00035124965,0.00012726929,0.00027348593,0.0000020503144],"about_ca_topic_score_codex":0.012920715,"about_ca_topic_score_gemma":0.014518424,"teacher_disagreement_score":0.012920715,"about_ca_system_score_codex":0.00055354025,"about_ca_system_score_gemma":0.00030955276,"threshold_uncertainty_score":0.025690973},"labels":[],"label_agreement":null},{"id":"W2005191849","doi":"10.1086/516627","title":"Propagating Star Formation in the Collisional Ring Galaxy Arp 10","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Spectroscopy; Spiral galaxy; RADIUS; Population; Astronomy; Star formation","score_opus":0.010037557722139613,"score_gpt":0.22783220807269758,"score_spread":0.21779465035055798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005191849","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991454,0.00003636231,0.00042314015,0.000006941993,0.0000011078921,0.0000032986777,0.0000125856195,0.000019835812,0.00035135716],"genre_scores_gemma":[0.99903834,0.000054946497,0.00070903316,0.0000048511038,0.0000024439173,0.0000049062282,0.00006081228,0.000005044071,0.00011951813],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998741,0.000031836513,0.0000049180276,0.00003740513,0.000024293044,0.000027408905],"domain_scores_gemma":[0.9997056,0.00004843415,0.0001224038,0.000035690835,0.0000196228,0.00006819844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022682028,0.0004269667,0.00029966517,0.0003559405,0.00037073635,0.0008971696,0.0007616276,0.00034952725,0.00036280445],"category_scores_gemma":[0.0005478371,0.00030153172,0.00035556435,0.00029958977,0.00054918963,0.00027518597,0.00050251844,0.00038002542,0.00010482988],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083325605,0.0007384937,0.3971951,0.000100947,0.00040685965,0.0023120975,0.0010159296,0.39874578,0.17275564,0.013597299,0.0005420418,0.011756539],"study_design_scores_gemma":[0.00013408586,0.00088543905,0.23283118,0.000015539857,0.00013710889,0.0008522793,0.00029847497,0.7482302,0.012664552,0.002290581,0.0015673916,0.000093211675],"about_ca_topic_score_codex":0.0068615354,"about_ca_topic_score_gemma":0.0022315132,"teacher_disagreement_score":0.0068615354,"about_ca_system_score_codex":0.0009289768,"about_ca_system_score_gemma":0.00022205593,"threshold_uncertainty_score":0.013643205},"labels":[],"label_agreement":null},{"id":"W2005214006","doi":"10.1088/0004-637x/757/2/108","title":"IONIZATION PARAMETER AS A DIAGNOSTIC OF RADIATION AND WIND PRESSURES IN H II REGIONS AND STARBURST GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Radiation pressure; Ionization; Adiabatic process; Radiation; Absorption (acoustics); Photon; Background radiation; Stars; Astronomy; Optics; Ion","score_opus":0.008728193341149585,"score_gpt":0.23314553298871873,"score_spread":0.22441733964756916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005214006","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99570364,0.00011273387,0.0019890503,0.000025668143,0.0000014645135,0.000008310299,0.00013641306,0.00008559924,0.0019370797],"genre_scores_gemma":[0.99921966,0.000021613492,0.0005673156,0.0000056637227,0.0000015227168,0.0000031753643,0.00006287338,0.000005156121,0.00011295321],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999926,0.000011517073,0.0000069919497,0.000017919134,0.000014038436,0.000023514016],"domain_scores_gemma":[0.99926084,0.00031850277,0.00023638077,0.000043889566,0.000026732765,0.00011378812],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021896303,0.00025405755,0.00015912205,0.0007632392,0.00020205468,0.00068269024,0.00034442917,0.0003515886,0.0009057382],"category_scores_gemma":[0.0013943837,0.00021771292,0.00023593081,0.0005453078,0.00049551233,0.00063721155,0.0005184915,0.00022916473,0.00012756744],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002047363,0.000055834826,0.87170583,0.000060482485,0.00005791127,0.00037684935,0.0005237477,0.0609561,0.046102997,0.008218004,0.00027064086,0.011466964],"study_design_scores_gemma":[0.000027746333,0.00013086673,0.85884947,0.000018676797,0.00002104837,0.0004520234,0.00043996488,0.12741596,0.007027203,0.004864163,0.0007279349,0.000024939842],"about_ca_topic_score_codex":0.0025307813,"about_ca_topic_score_gemma":0.001799967,"teacher_disagreement_score":0.0025307813,"about_ca_system_score_codex":0.0004721113,"about_ca_system_score_gemma":0.00013802384,"threshold_uncertainty_score":0.0050320625},"labels":[],"label_agreement":null},{"id":"W2005268336","doi":"10.1086/511977","title":"ACS Photometry of Newly Discovered Globular Clusters in the Outer Halo of M31","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Photometry (optics); Astrophysics; Physics; Milky Way; Halo; Astronomy; Galaxy; Horizontal branch; Andromeda Galaxy; Stars","score_opus":0.010308549760399695,"score_gpt":0.2409270068672448,"score_spread":0.23061845710684512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005268336","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99829715,0.00010081023,0.00023651388,0.000019277675,0.0000021162787,0.000008205993,0.00026712217,0.000025524334,0.0010432662],"genre_scores_gemma":[0.9970342,0.0000804746,0.0010991237,0.000024690775,0.000014084462,0.000009398914,0.0012589503,0.000012328967,0.00046663266],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997745,0.00001236401,0.000011407326,0.0000437431,0.00010049267,0.00005744326],"domain_scores_gemma":[0.99927634,0.00005657272,0.00013665142,0.00008421091,0.00016946754,0.00027677865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003064189,0.0002715626,0.00021756765,0.0015570045,0.00056590454,0.0006485571,0.00037649088,0.00024257165,0.0006684303],"category_scores_gemma":[0.00073149643,0.00024792945,0.00023461539,0.0010275372,0.00033375729,0.00035017479,0.0010750367,0.00023340853,0.00032958633],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002528,0.00006378857,0.88504606,0.00006478463,0.00008320995,0.0005309708,0.0013680408,0.002575181,0.088760816,0.0006963663,0.0014471076,0.019110804],"study_design_scores_gemma":[0.0000090474905,0.000038574748,0.99500173,0.000005935385,0.00001274236,0.00018526884,0.00014864128,0.0015567812,0.0014584701,0.00013795691,0.0014350641,0.000009673818],"about_ca_topic_score_codex":0.012386206,"about_ca_topic_score_gemma":0.02741648,"teacher_disagreement_score":0.012386206,"about_ca_system_score_codex":0.0007124878,"about_ca_system_score_gemma":0.00030293473,"threshold_uncertainty_score":0.024628222},"labels":[],"label_agreement":null},{"id":"W2005286960","doi":"10.1086/508917","title":"Corona of Magnetars","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":350,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Corona (planetary geology); Magnetosphere; Magnetar; Corona ring; Electric field; Plasma; Magnetohydrodynamics; Magnetic field; Nanoflares","score_opus":0.010862855977299907,"score_gpt":0.31579452176597184,"score_spread":0.3049316657886719,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005286960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.42218474,0.003532201,0.28667447,0.006779156,0.0008394003,0.00031104128,0.0012928483,0.0009397597,0.27744648],"genre_scores_gemma":[0.9494625,0.0009595267,0.01641707,0.00078826287,0.00022076501,0.00022251772,0.00039022957,0.000082707644,0.031456474],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99991107,0.000019750194,0.0000030867643,0.00002527257,0.00002022384,0.000020545493],"domain_scores_gemma":[0.9998846,0.000021161486,0.000022310564,0.000014759875,0.000034977544,0.000022207949],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015316083,0.0003877213,0.00046677105,0.0003803462,0.00080644357,0.0009960158,0.001166703,0.0012685577,0.00774848],"category_scores_gemma":[0.0005723376,0.00023128385,0.000652457,0.00022581579,0.00058493554,0.0012405312,0.00064126664,0.00048972125,0.0011054602],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000100817524,0.00012452519,0.004618711,0.00018915314,0.000082020044,0.0009343524,0.00036586102,0.29599106,0.011777151,0.66478974,0.008626633,0.012400009],"study_design_scores_gemma":[0.0001280126,0.00016618168,0.003945417,0.0000327608,0.000048713096,0.00061236706,0.00020035706,0.8021123,0.0012098084,0.16652887,0.02497841,0.000036803445],"about_ca_topic_score_codex":0.0028787835,"about_ca_topic_score_gemma":0.0013995123,"teacher_disagreement_score":0.00774848,"about_ca_system_score_codex":0.0007729867,"about_ca_system_score_gemma":0.00044832285,"threshold_uncertainty_score":0.025921285},"labels":[],"label_agreement":null},{"id":"W2005300162","doi":"10.1086/429126","title":"Properties of the Hα‐emitting Circumstellar Regions of Be Stars","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"U.S. Naval Observatory; Office of Naval Research; National Aeronautics and Space Administration; Government of Ontario; California Institute of Technology; Jet Propulsion Laboratory; University of Toronto","keywords":"Stars; Astrophysics; Circumstellar disk; Physics; Astronomy","score_opus":0.020051073414937223,"score_gpt":0.21495975233487302,"score_spread":0.1949086789199358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005300162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988662,0.00016227025,0.00047601748,0.0000044214703,7.8314076e-7,0.0000019454812,0.000120518875,0.000011428722,0.0003563328],"genre_scores_gemma":[0.999003,0.00011450096,0.00028606586,0.0000052157584,0.0000041683275,0.000002413872,0.0004739126,0.0000043016653,0.00010635201],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.0000072506828,0.0000060018615,0.000016393029,0.000012022231,0.000012078843],"domain_scores_gemma":[0.9995927,0.000080434496,0.00017390827,0.000030484394,0.000053358748,0.000069119014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015614381,0.0002498354,0.00020773963,0.0006020708,0.0002732763,0.00033903553,0.00017644273,0.00018764762,0.00045504578],"category_scores_gemma":[0.000510654,0.00013390012,0.00016273657,0.0005704122,0.0001971072,0.00028759483,0.00019335213,0.00013477361,0.00017627154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005831361,0.00008109175,0.78506345,0.00008587439,0.00012449049,0.0005324118,0.0004011815,0.001871521,0.19294152,0.00028904947,0.0001196654,0.017906554],"study_design_scores_gemma":[0.00000519555,0.00012230064,0.99254006,0.0000027464687,0.00002202364,0.0009130479,0.00008219064,0.0013592377,0.0044302437,0.00013770789,0.00038033142,0.0000049179075],"about_ca_topic_score_codex":0.0006308913,"about_ca_topic_score_gemma":0.000546083,"teacher_disagreement_score":0.0006308913,"about_ca_system_score_codex":0.00010777975,"about_ca_system_score_gemma":0.00004780818,"threshold_uncertainty_score":0.0015223026},"labels":[],"label_agreement":null},{"id":"W2005370037","doi":"10.1088/0004-637x/797/2/129","title":"QUANTIFYING THE HEATING SOURCES FOR MID-INFRARED DUST EMISSIONS IN GALAXIES: THE CASE OF M 81","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Emissivity; Emission spectrum; Radiation; Thermal emission; Cosmic dust; Spire (mollusc); Galaxy; Ionization","score_opus":0.02735813648290027,"score_gpt":0.2858959966722801,"score_spread":0.25853786018937985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005370037","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994795,0.00007319833,0.00012038925,0.000005804544,2.506904e-7,0.0000015718632,0.000044120778,0.0000044934186,0.00027066175],"genre_scores_gemma":[0.99963355,0.000048625912,0.00017849171,0.000002079895,0.0000019664033,0.0000017909169,0.00008138991,0.0000013521517,0.000050603954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998317,0.000023618524,0.0000109736875,0.00006215553,0.000030516963,0.000041004678],"domain_scores_gemma":[0.9992434,0.00019141835,0.00031487728,0.0001388021,0.000046652778,0.00006486357],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022624662,0.0002709463,0.00023976868,0.0015424165,0.00023436699,0.00062422693,0.00037886683,0.00031629697,0.00038811937],"category_scores_gemma":[0.0012330154,0.00017942699,0.00030758587,0.0009883549,0.0004943855,0.0005252052,0.0006888955,0.00015017482,0.00018312057],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007910299,0.000018663794,0.9841966,0.000016806041,0.000042615684,0.00031945098,0.00027089508,0.0012597545,0.0100104865,0.00020807002,0.000030685296,0.0035468058],"study_design_scores_gemma":[0.000001487875,0.000014027938,0.9975643,0.000002070623,0.000014851922,0.000108470085,0.000118748365,0.0013333578,0.0006903312,0.00006152892,0.00008790443,0.000002958121],"about_ca_topic_score_codex":0.0064546335,"about_ca_topic_score_gemma":0.0091470005,"teacher_disagreement_score":0.0064546335,"about_ca_system_score_codex":0.0005684507,"about_ca_system_score_gemma":0.00015715368,"threshold_uncertainty_score":0.012834132},"labels":[],"label_agreement":null},{"id":"W2005370313","doi":"10.1086/508650","title":"Quasars: What Turns Them Off?","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Canadian Institute for Theoretical Astrophysics; Queen's University","funders":"","keywords":"Quasar; Astrophysics; Physics; Redshift; Galaxy; Luminosity function; Luminosity; Astronomy; Halo; Galaxy formation and evolution; Dark matter; OVV quasar","score_opus":0.008477732845067091,"score_gpt":0.20635920257109602,"score_spread":0.19788146972602894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005370313","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.71420884,0.026314324,0.03385911,0.035351615,0.0040012505,0.00005834852,0.003604422,0.0025320451,0.18007001],"genre_scores_gemma":[0.9739811,0.003109081,0.0032120107,0.0028622618,0.0004557262,0.000011236284,0.0003881686,0.00013517562,0.015845345],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","domain_scores_codex":[0.99995863,0.0000073931396,0.000001367223,0.000008848717,0.000011709002,0.00001207563],"domain_scores_gemma":[0.99990284,0.000024981098,0.000024614075,0.0000109697385,0.000012823078,0.000023813862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000093485054,0.00019199614,0.00016098683,0.00028422405,0.00020463564,0.00091166334,0.00030622672,0.00036817332,0.008619565],"category_scores_gemma":[0.0006292531,0.00006956315,0.00021500947,0.00026108924,0.00048891176,0.0007145113,0.00030225847,0.0003348677,0.0013053636],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041531638,0.00012511006,0.10445425,0.0005622533,0.00014841533,0.0021409579,0.0018116555,0.037914094,0.011433521,0.34948313,0.15564632,0.335865],"study_design_scores_gemma":[0.00014686736,0.00034603925,0.1780699,0.00027379938,0.000105961895,0.0019965628,0.0020239986,0.04931733,0.005402431,0.39635727,0.3658741,0.00008585345],"about_ca_topic_score_codex":0.003645249,"about_ca_topic_score_gemma":0.004129873,"teacher_disagreement_score":0.008619565,"about_ca_system_score_codex":0.00028353793,"about_ca_system_score_gemma":0.0001124343,"threshold_uncertainty_score":0.028835356},"labels":[],"label_agreement":null},{"id":"W2005621462","doi":"10.1088/0004-637x/768/2/131","title":"THE BURST MODE OF ACCRETION IN PRIMORDIAL PROTOSTARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Protostar; Accretion (finance); Gravitational instability; Accretion disc; Gravitational collapse; Stars; Solar mass; Stellar evolution; Fragmentation (computing)","score_opus":0.0074934391702025285,"score_gpt":0.24171851688259496,"score_spread":0.23422507771239243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005621462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99641377,0.000121671226,0.002592051,0.000051143124,0.00000725482,0.0000065585546,0.000053715583,0.000039891318,0.00071401044],"genre_scores_gemma":[0.99890757,0.00006831454,0.0007053633,0.00001228482,0.0000048692305,0.000006162744,0.000049303053,0.000010120088,0.0002358503],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999461,0.000010022787,0.00000248675,0.000014388068,0.000008929078,0.000018013734],"domain_scores_gemma":[0.99971575,0.00007158121,0.00008991525,0.000019614261,0.000025213785,0.000077880206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023371362,0.0003695912,0.00036843296,0.00032558915,0.00041418933,0.00059685734,0.00056786725,0.00058653054,0.00051325915],"category_scores_gemma":[0.0010776422,0.00023755032,0.00039450548,0.00020704478,0.00061010866,0.0004657466,0.00050594803,0.00039253166,0.00009108051],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005212137,0.00020017593,0.18737827,0.00014753081,0.00023186755,0.0017854684,0.00092460314,0.73745126,0.046984896,0.016117882,0.0009203268,0.0073366147],"study_design_scores_gemma":[0.00008467939,0.00009525964,0.023475546,0.000010518926,0.000027334438,0.00017786172,0.00011935002,0.9694248,0.0027891113,0.0032761984,0.0005008338,0.000018499304],"about_ca_topic_score_codex":0.0053343177,"about_ca_topic_score_gemma":0.0019575544,"teacher_disagreement_score":0.0053343177,"about_ca_system_score_codex":0.0005511364,"about_ca_system_score_gemma":0.0003642147,"threshold_uncertainty_score":0.010606527},"labels":[],"label_agreement":null},{"id":"W2005639341","doi":"10.1086/499485","title":"The ACS Virgo Cluster Survey. XI. The Nature of Diffuse Star Clusters in Early‐Type Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Virgo Cluster; Globular cluster; Astronomy; Elliptical galaxy; Surface brightness; Star cluster; Galaxy cluster; Galaxy","score_opus":0.0055199332039230446,"score_gpt":0.20756814349871586,"score_spread":0.2020482102947928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005639341","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14789626,0.0021774562,0.0013903196,0.00061132165,0.00006534439,0.00029645968,0.80342126,0.0023113738,0.04183026],"genre_scores_gemma":[0.17077698,0.0019301124,0.0045275465,0.00037292537,0.00009388401,0.00022182422,0.8054548,0.0003607476,0.016261145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997924,0.000018546116,0.00001461541,0.000050706738,0.00007318313,0.000050471106],"domain_scores_gemma":[0.99941266,0.000040057726,0.00017195809,0.0000760458,0.00013269403,0.00016667211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004058623,0.0005361302,0.00042538837,0.005045917,0.00029677397,0.00080348505,0.0006058539,0.00031164155,0.012995176],"category_scores_gemma":[0.00071071065,0.00023453441,0.00024063667,0.0059333607,0.00013434839,0.0005224765,0.0008086968,0.0003473081,0.011532666],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045810128,0.00020587769,0.49470016,0.0005940906,0.00032131321,0.00032088114,0.000421093,0.0006471693,0.0064088707,0.0025564756,0.3943299,0.099036135],"study_design_scores_gemma":[0.0000869925,0.00003759474,0.87360406,0.00006244473,0.000053000753,0.00020463165,0.00015765698,0.00068818737,0.0007163664,0.0005244671,0.123848364,0.000016286294],"about_ca_topic_score_codex":0.026574293,"about_ca_topic_score_gemma":0.026728895,"teacher_disagreement_score":0.026574293,"about_ca_system_score_codex":0.0006015664,"about_ca_system_score_gemma":0.00038584892,"threshold_uncertainty_score":0.05283922},"labels":[],"label_agreement":null},{"id":"W2005643987","doi":"10.1086/589178","title":"The Damping Rates of Embedded Oscillating Starless Cores","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Oscillation (cell signaling); Perturbation (astronomy); Formalism (music); Excitation; Astrophysics; Spectral line; Classical mechanics; Mechanics; Astronomy; Quantum mechanics","score_opus":0.023570206454218107,"score_gpt":0.27172899421128777,"score_spread":0.24815878775706965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005643987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99254346,0.00009972712,0.006927843,0.000016333206,0.0000042731995,0.000005132271,0.000013473436,0.000040338036,0.0003495004],"genre_scores_gemma":[0.999186,0.000025080233,0.0005995209,0.0000023107252,0.0000017960695,0.0000020664,0.000015248869,0.00000949733,0.00015854719],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999474,0.0000069678763,0.0000030103204,0.000016439202,0.000014809053,0.000011379753],"domain_scores_gemma":[0.99945277,0.00018066881,0.00017822334,0.000045103796,0.00006900581,0.000074209216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017555716,0.00022582033,0.00018179767,0.00037960234,0.00015496198,0.0002875394,0.0003310532,0.00017982505,0.00064121315],"category_scores_gemma":[0.0016097748,0.00017137942,0.00014743656,0.00008980626,0.000363395,0.00040225088,0.00044978684,0.00030468302,0.00012432218],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005428823,0.000104725914,0.06780493,0.00018413777,0.00007897734,0.0010344695,0.0013751193,0.09610502,0.79115987,0.011462448,0.00032606954,0.029821431],"study_design_scores_gemma":[0.000063656196,0.00043744632,0.07677455,0.000020291409,0.000050585302,0.00076825224,0.000258052,0.73306566,0.17972541,0.007332701,0.0014354226,0.00006792834],"about_ca_topic_score_codex":0.00037679984,"about_ca_topic_score_gemma":0.0001794417,"teacher_disagreement_score":0.00064121315,"about_ca_system_score_codex":0.00018171448,"about_ca_system_score_gemma":0.00005717685,"threshold_uncertainty_score":0.0021451116},"labels":[],"label_agreement":null},{"id":"W2005653912","doi":"10.1088/0004-637x/781/2/104","title":"SDSS J074511.56+194926.5: DISCOVERY OF A METAL-RICH AND TIDALLY DISTORTED EXTREMELY LOW MASS WHITE DWARF","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Astrophysics Division; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"White dwarf; Astrophysics; Metallicity; Physics; Surface gravity; Balmer series; Solar mass; Radial velocity; Low Mass; Mass ratio; Orbital period; Astronomy; Spectral line; Stars; Emission spectrum","score_opus":0.008210257267193677,"score_gpt":0.20315480595706667,"score_spread":0.194944548689873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005653912","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9847936,0.00052440254,0.00083581364,0.00058209937,0.000089612935,0.00004282501,0.004041216,0.0003080952,0.008782371],"genre_scores_gemma":[0.9709928,0.00032888676,0.0038674541,0.0010389306,0.00024757878,0.000034928806,0.018474111,0.000086311324,0.0049290573],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997712,0.0000125977185,0.000025210302,0.0000632604,0.00007949878,0.000048225025],"domain_scores_gemma":[0.9994455,0.000023981424,0.00016914745,0.000051481686,0.0000640582,0.0002457389],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006104288,0.00035888643,0.00044403187,0.002054854,0.00085660233,0.0009893416,0.00049492746,0.0007448036,0.0015766271],"category_scores_gemma":[0.00047303838,0.000181397,0.00015098348,0.0013538083,0.0003133397,0.00033353147,0.00094282924,0.00040476077,0.0012504673],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081003306,0.00056743115,0.73866457,0.00031691263,0.00024267734,0.021548135,0.0012572015,0.00069556443,0.1438575,0.0035493919,0.03306955,0.055421],"study_design_scores_gemma":[0.00007188567,0.00018849614,0.9396391,0.000029586992,0.00006371165,0.00860593,0.00036131425,0.0020156018,0.0053300643,0.0008536133,0.042802006,0.000038615588],"about_ca_topic_score_codex":0.0037107768,"about_ca_topic_score_gemma":0.009075203,"teacher_disagreement_score":0.0037107768,"about_ca_system_score_codex":0.000584375,"about_ca_system_score_gemma":0.00031938896,"threshold_uncertainty_score":0.00737834},"labels":[],"label_agreement":null},{"id":"W2005674604","doi":"10.1086/512181","title":"The Evolution of Very Massive Stars","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Stars; Physics; Supernova; Astrophysics; Stellar evolution; Gravitational collapse; Stellar collision; Instability; Astronomy; Mechanics","score_opus":0.007111506026843422,"score_gpt":0.21918278435803387,"score_spread":0.21207127833119044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005674604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8828125,0.001382159,0.085686944,0.00031664752,0.00010601287,0.000036350462,0.00017792937,0.00026467894,0.029216787],"genre_scores_gemma":[0.9726819,0.000532655,0.019422922,0.00006963917,0.000031804666,0.000016298078,0.0001359694,0.000060952047,0.0070478674],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999232,0.000016141863,0.0000034772236,0.000017585122,0.00002780393,0.000011766516],"domain_scores_gemma":[0.9998611,0.000024654864,0.000036216603,0.000025473715,0.000022272157,0.000030182604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017332785,0.00018392377,0.00017276681,0.00023456705,0.00050974847,0.0005278302,0.00051747833,0.0005000884,0.0009853302],"category_scores_gemma":[0.00076358253,0.00018770272,0.0003725182,0.00021783459,0.00047611835,0.00048305088,0.00090043986,0.0003327118,0.00025494298],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014244924,0.00010588653,0.050874956,0.00021070529,0.00010239236,0.0013996452,0.0007870384,0.2927207,0.07244771,0.5116283,0.0027761597,0.06680413],"study_design_scores_gemma":[0.000071469534,0.00019738622,0.08357381,0.000075268414,0.00006315971,0.002264237,0.00021915046,0.6244157,0.018271333,0.22928803,0.041452367,0.00010815543],"about_ca_topic_score_codex":0.002010854,"about_ca_topic_score_gemma":0.0012345726,"teacher_disagreement_score":0.002010854,"about_ca_system_score_codex":0.0005146406,"about_ca_system_score_gemma":0.00030490907,"threshold_uncertainty_score":0.003998339},"labels":[],"label_agreement":null},{"id":"W2005851202","doi":"10.1088/0004-637x/801/2/143","title":"DOES THE PRESENCE OF PLANETS AFFECT THE FREQUENCY AND PROPERTIES OF EXTRASOLAR KUIPER BELTS? RESULTS FROM THE<i>HERSCHEL</i>DEBRIS AND DUNES SURVEYS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Planet; Debris disk; Exoplanet; Stars; Planetary system; Metallicity; Debris; Astrophysics; Astronomy; Planetary migration; Astrobiology","score_opus":0.019815690069445155,"score_gpt":0.2115595714732343,"score_spread":0.19174388140378912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005851202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989876,0.00018675844,0.000050387116,0.00005726699,0.000003797821,0.0000020195482,0.00025580882,0.0000034125492,0.00045286067],"genre_scores_gemma":[0.9995383,0.000049783463,0.000023787208,0.000018158069,0.00000815791,0.000001211437,0.00019438981,0.0000027752399,0.00016349122],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994035,0.00015399611,0.000055756405,0.00019723525,0.00006532082,0.00012419948],"domain_scores_gemma":[0.9932747,0.0016201135,0.0034347936,0.00068758463,0.00028953567,0.0006933694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00070410664,0.00022330179,0.00031732663,0.0010224924,0.00039716708,0.00083692133,0.0005019662,0.00073178957,0.0026453452],"category_scores_gemma":[0.004388145,0.00019644394,0.0005118813,0.0008293233,0.00061682047,0.0006908341,0.00048564604,0.0003566055,0.0007011373],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000028588185,0.000008627595,0.99889225,0.0000038624867,0.000030392346,0.000026338326,0.000053106894,0.000017255266,0.0003305566,0.000005799142,0.000022875629,0.0005803707],"study_design_scores_gemma":[4.7502212e-7,0.000009437952,0.9998367,8.077217e-7,0.0000046895884,0.000024927615,0.000037415644,0.000014099679,0.000024776687,0.0000037034845,0.0000423357,6.036496e-7],"about_ca_topic_score_codex":0.0074152458,"about_ca_topic_score_gemma":0.009906465,"teacher_disagreement_score":0.0074152458,"about_ca_system_score_codex":0.00022337974,"about_ca_system_score_gemma":0.00012445182,"threshold_uncertainty_score":0.014744163},"labels":[],"label_agreement":null},{"id":"W2005923494","doi":"10.1086/342526","title":"Angular Momentum Extraction by Gravity Waves in the Sun","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":147,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Compute Canada","funders":"","keywords":"Angular momentum; Physics; Convection zone; Radiation zone; Radiative transfer; Convection; Gravity wave; Gravitational wave; Helioseismology; Momentum (technical analysis); Mechanics; Classical mechanics; Geophysics; Astrophysics; Optics","score_opus":0.007785454846951416,"score_gpt":0.22654651010916152,"score_spread":0.2187610552622101,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2005923494","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7468233,0.13342865,0.037797473,0.00092907663,0.0011874683,0.000034711098,0.00016427453,0.00040833667,0.07922667],"genre_scores_gemma":[0.95670176,0.031680517,0.0025572185,0.000116061674,0.0004771079,0.000011244476,0.00006819837,0.000052590116,0.008335437],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996054,0.0000041703056,0.0000019666713,0.00001176985,0.000012331369,0.000009371678],"domain_scores_gemma":[0.999969,0.000007803887,0.000009623409,0.0000028016668,0.000006140214,0.0000045078596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007898793,0.00026586096,0.00025374358,0.00025616732,0.0002340847,0.00050144305,0.00012704097,0.00024412572,0.0008051524],"category_scores_gemma":[0.000210316,0.0001308837,0.00017946858,0.0001867359,0.00023335313,0.00053807354,0.00029743795,0.00024883245,0.000318156],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005198433,0.000086447675,0.017558774,0.001317106,0.00019812834,0.0022092625,0.0011272811,0.04714748,0.46585867,0.23190264,0.007750062,0.2243243],"study_design_scores_gemma":[0.0001411815,0.0014232341,0.117206775,0.00046651895,0.00026200095,0.0057755527,0.0005769925,0.11586598,0.13734789,0.3088091,0.31180683,0.0003179407],"about_ca_topic_score_codex":0.00035679052,"about_ca_topic_score_gemma":0.00016379735,"teacher_disagreement_score":0.0008051524,"about_ca_system_score_codex":0.00021740944,"about_ca_system_score_gemma":0.00006703769,"threshold_uncertainty_score":0.0026934743},"labels":[],"label_agreement":null},{"id":"W2006147525","doi":"10.1088/0004-637x/730/1/11","title":"STAR FORMATION IN DISK GALAXIES. II. THE EFFECT OF STAR FORMATION AND PHOTOELECTRIC HEATING ON THE FORMATION AND EVOLUTION OF GIANT MOLECULAR CLOUDS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Star formation; Astrophysics; Molecular cloud; Milky Way; Galaxy; Population; Astronomy; Interstellar medium; Stars; Fragmentation (computing); Galaxy formation and evolution","score_opus":0.007256910318838145,"score_gpt":0.20630266501091005,"score_spread":0.1990457546920719,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006147525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986779,0.00031761682,0.00021918537,0.00004439647,0.0000035339503,0.0000037393863,0.00009770573,0.000009485217,0.00062632735],"genre_scores_gemma":[0.99944884,0.00012223051,0.0001443956,0.00001410666,0.000002902425,0.0000024363235,0.00008725829,0.000003946639,0.00017395937],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999163,0.000022001765,0.000005014598,0.00001886381,0.000010913831,0.00002680058],"domain_scores_gemma":[0.99966633,0.00008927521,0.00008910279,0.000041861407,0.000025440035,0.000087988155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021199933,0.00025549484,0.00024468917,0.00020539782,0.00024371824,0.000596708,0.00038188157,0.00044256425,0.0011983624],"category_scores_gemma":[0.0008392771,0.00019545651,0.0004413608,0.0002192488,0.000420277,0.00040685403,0.0004846446,0.00029245517,0.00020369444],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044838997,0.00014012629,0.6955449,0.00019398305,0.0003430461,0.0003386987,0.00040642702,0.26509753,0.02484819,0.0029985916,0.0005830543,0.00905707],"study_design_scores_gemma":[0.00014679068,0.00048112412,0.7885682,0.000036872552,0.000119601355,0.000306515,0.00043482156,0.19882405,0.004967118,0.0036721833,0.0024122347,0.000030387713],"about_ca_topic_score_codex":0.0062384,"about_ca_topic_score_gemma":0.0064463066,"teacher_disagreement_score":0.0062384,"about_ca_system_score_codex":0.0006044267,"about_ca_system_score_gemma":0.00017503666,"threshold_uncertainty_score":0.012404203},"labels":[],"label_agreement":null},{"id":"W2006165287","doi":"10.1086/499769","title":"Early Cosmic Chemical Evolution: Relating the Origin of a Diffuse Intergalactic Medium and the First Long‐Lived Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supernova; Astrophysics; Stars; Physics; Galaxy; Redshift; Intergalactic medium; Star formation; Galaxy formation and evolution; Baryon; COSMIC cancer database; Astronomy","score_opus":0.005874919194647645,"score_gpt":0.19836355247980975,"score_spread":0.1924886332851621,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006165287","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974879,0.0008468056,0.0002672332,0.00006434862,0.0000034262018,0.0000026681428,0.00010180717,0.0000045482266,0.0012211462],"genre_scores_gemma":[0.9990325,0.00041282224,0.00016311002,0.000020907966,0.000008427514,0.0000011961856,0.000114615454,0.0000015455217,0.00024484852],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996555,0.0000070519277,0.0000015908315,0.000009669723,0.000007221253,0.000008867582],"domain_scores_gemma":[0.9996619,0.000062197505,0.0001262992,0.000029056268,0.000034411907,0.00008601554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017574742,0.00017809529,0.000078074016,0.0007218211,0.0001791803,0.0007203614,0.00018979485,0.00033922723,0.00079215405],"category_scores_gemma":[0.0006725707,0.00010146193,0.00010032962,0.00075695594,0.00041268993,0.00048650507,0.00041044792,0.00031069815,0.00010954577],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001554178,0.00004605744,0.96967274,0.00004774368,0.00007603357,0.00023020971,0.00022181487,0.00047972045,0.011930174,0.0024851304,0.00011024882,0.014544589],"study_design_scores_gemma":[0.0000018560519,0.000019112827,0.99783915,0.000004468921,0.000014013628,0.00020197348,0.000077892895,0.0002633864,0.0006741624,0.00057767896,0.00032391245,0.0000023854393],"about_ca_topic_score_codex":0.003866892,"about_ca_topic_score_gemma":0.0065090507,"teacher_disagreement_score":0.003866892,"about_ca_system_score_codex":0.00048606726,"about_ca_system_score_gemma":0.0001528928,"threshold_uncertainty_score":0.0076887608},"labels":[],"label_agreement":null},{"id":"W2006246655","doi":"10.1086/429913","title":"A Safety Net for Fast Migrators: Interactions between Gap‐opening and Sub–Gap‐opening Bodies in a Protoplanetary Disk","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Protoplanet; Planet; Giant planet; Gas giant; Protoplanetary disk; Angular momentum; Dissipative system; Planetary system; Accretion (finance)","score_opus":0.018192257834508584,"score_gpt":0.2676875939025146,"score_spread":0.24949533606800603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006246655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9714739,0.000081995306,0.023367401,0.00031869562,0.00003435655,0.000042471962,0.00013296895,0.00038445878,0.004163751],"genre_scores_gemma":[0.9874449,0.000045897326,0.010807877,0.000042567677,0.000009487459,0.00003517711,0.000112042275,0.000074154435,0.0014277954],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992764,0.000017874516,0.0000038656203,0.000013859646,0.000023321836,0.00001347484],"domain_scores_gemma":[0.999373,0.00030355187,0.00011540729,0.000051661,0.000061782855,0.00009447886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029499875,0.00031941244,0.00023035183,0.00028116687,0.0008296311,0.00086483685,0.00079259236,0.00090299116,0.002661581],"category_scores_gemma":[0.001937448,0.0002629862,0.00019162579,0.00014418285,0.0007241468,0.00081471517,0.0011304165,0.0005098218,0.00022757088],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048229148,0.00030068395,0.06424254,0.00014335707,0.000046161425,0.0008103592,0.0008584215,0.8542791,0.023896227,0.027483555,0.0021803775,0.02527698],"study_design_scores_gemma":[0.000036095033,0.000065113716,0.0026407212,0.000008085604,0.0000062495906,0.00006608691,0.00011457322,0.9915809,0.0021439614,0.0023812545,0.00094917347,0.000007769683],"about_ca_topic_score_codex":0.0039157327,"about_ca_topic_score_gemma":0.0027223341,"teacher_disagreement_score":0.0039157327,"about_ca_system_score_codex":0.0003859477,"about_ca_system_score_gemma":0.00077864603,"threshold_uncertainty_score":0.008903921},"labels":[],"label_agreement":null},{"id":"W2006277953","doi":"10.1086/509862","title":"The Extinction and Distance of Maffei 2 and a New View of the IC 342/Maffei Group","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Extinction (optical mineralogy); Spiral galaxy; Galaxy; Milky Way; Interstellar medium; Galaxy group","score_opus":0.006094035860683028,"score_gpt":0.20595285674362387,"score_spread":0.19985882088294085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006277953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996077,0.00039924242,0.00089291367,0.00006932852,0.000007906274,0.0000041934795,0.000027263679,0.000020153788,0.002502054],"genre_scores_gemma":[0.9980286,0.00010808965,0.0010979391,0.000033813696,0.000032461114,0.0000044077133,0.000085640364,0.0000071842414,0.0006019154],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982077,0.000022813392,0.000005596535,0.000051471063,0.000038336962,0.00006101484],"domain_scores_gemma":[0.99957186,0.00003536249,0.00011855115,0.00006688686,0.00007744597,0.00012985799],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045586395,0.00033568087,0.00020982105,0.001664566,0.00042220292,0.00067833654,0.00039468022,0.0004326276,0.00092428166],"category_scores_gemma":[0.0010289566,0.00022982006,0.00022486487,0.00044492885,0.00047121884,0.0005445749,0.0006185728,0.00042594265,0.00020971824],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033792167,0.00008562302,0.88012624,0.000045291185,0.00008139789,0.0009120988,0.0018212713,0.0010638371,0.079022944,0.0022286908,0.00059684814,0.033677716],"study_design_scores_gemma":[0.000013226128,0.000094323914,0.9896666,0.000012686371,0.000028409417,0.0007193864,0.00021376651,0.0014768919,0.0027392595,0.00093746476,0.004077454,0.000020610598],"about_ca_topic_score_codex":0.005278975,"about_ca_topic_score_gemma":0.006684282,"teacher_disagreement_score":0.005278975,"about_ca_system_score_codex":0.0004425143,"about_ca_system_score_gemma":0.00013741739,"threshold_uncertainty_score":0.010496497},"labels":[],"label_agreement":null},{"id":"W2006287789","doi":"10.1086/588781","title":"Large Excess of Heavy Nitrogen in Both Hydrogen Cyanide and Cyanogen from Comet 17P/Holmes","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; National Aeronautics and Space Administration; California Institute of Technology; University of Texas at Austin; W. M. Keck Foundation; Fonds De La Recherche Scientifique - FNRS","keywords":"Cyanogen; Comet; Formation and evolution of the Solar System; Nitrogen; Solar System; Astrobiology; Hydrogen cyanide; Jupiter (rocket family); Hydrogen; Fractionation; Stratosphere; Chemistry; Physics; Astrophysics; Astronomy; Atmospheric sciences; Inorganic chemistry; Organic chemistry","score_opus":0.010145759544387204,"score_gpt":0.21211311902948138,"score_spread":0.20196735948509417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006287789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990951,0.00017428961,0.000060997307,0.00001151656,0.000003533303,0.0000014632436,0.00018905071,0.000004601533,0.00045953412],"genre_scores_gemma":[0.9983695,0.00012243808,0.00014945221,0.000024627385,0.000008123511,0.0000030014685,0.0009632931,0.0000064417623,0.00035316532],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998889,0.0000036487866,0.0000046333475,0.00004463581,0.00003545317,0.000022808528],"domain_scores_gemma":[0.999861,0.000013924247,0.00004760759,0.0000145374515,0.000028743803,0.000034215656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001139997,0.00021631912,0.00021723124,0.0006877705,0.00046359526,0.00043684046,0.0002600515,0.00025273554,0.0006108796],"category_scores_gemma":[0.00020521595,0.00016125492,0.00012262851,0.000338477,0.0002872112,0.00030171117,0.00040117363,0.00018411291,0.00015940421],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005198674,0.000029155786,0.31450155,0.0000649191,0.000095471776,0.001471875,0.00029458816,0.000114089235,0.6763743,0.00008970746,0.00014471884,0.006299696],"study_design_scores_gemma":[0.000014665742,0.00010374532,0.9472688,0.0000064922933,0.00005311152,0.0011012128,0.00023698217,0.00034072885,0.049598597,0.00006129093,0.0012060846,0.000008241852],"about_ca_topic_score_codex":0.009284096,"about_ca_topic_score_gemma":0.011598176,"teacher_disagreement_score":0.009284096,"about_ca_system_score_codex":0.0005269799,"about_ca_system_score_gemma":0.0001626404,"threshold_uncertainty_score":0.018460155},"labels":[],"label_agreement":null},{"id":"W2006305466","doi":"10.1088/0004-637x/732/2/76","title":"PAndAS’ PROGENY: EXTENDING THE M31 DWARF GALAXY CABAL","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":182,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Dwarf spheroidal galaxy; Dwarf galaxy; Astrophysics; Local Group; Red-giant branch; Galaxy; Dwarf galaxy problem; Astronomy; Satellite galaxy; Andromeda; Stars; Andromeda Galaxy; Globular cluster; Milky Way; Interacting galaxy","score_opus":0.01671583431017154,"score_gpt":0.22117289206544016,"score_spread":0.20445705775526862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006305466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8915764,0.0018232485,0.002533844,0.0014357537,0.00012221947,0.0000561698,0.0025745365,0.00073472946,0.09914313],"genre_scores_gemma":[0.9843859,0.00042183965,0.0038382956,0.00028603047,0.000054611533,0.000020697622,0.0021961525,0.00008654576,0.008709895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998148,0.000020136333,0.0000043225386,0.0000657069,0.000045454115,0.00004961913],"domain_scores_gemma":[0.9996525,0.000045102268,0.000047943446,0.00008504636,0.000082650244,0.00008674485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026109745,0.00016193074,0.000113446426,0.0007578943,0.0012356596,0.0007366011,0.00029967693,0.00021916708,0.0050210166],"category_scores_gemma":[0.0007312357,0.00011350486,0.0001463326,0.000507917,0.00045933985,0.00049682806,0.0009757552,0.0003003184,0.0014740812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007656249,0.00015364429,0.5085997,0.00019098239,0.000065202614,0.003077816,0.004779029,0.00059312896,0.019152235,0.029468725,0.035889342,0.39726472],"study_design_scores_gemma":[0.000025599207,0.00016224253,0.39812285,0.00004764825,0.000025918209,0.0050962204,0.0012335224,0.00090710213,0.0031277288,0.003307837,0.5879097,0.000033664164],"about_ca_topic_score_codex":0.022508418,"about_ca_topic_score_gemma":0.026277162,"teacher_disagreement_score":0.022508418,"about_ca_system_score_codex":0.0005777466,"about_ca_system_score_gemma":0.00059591146,"threshold_uncertainty_score":0.044754803},"labels":[],"label_agreement":null},{"id":"W2006321533","doi":"10.1088/0004-637x/748/1/25","title":"MOLECULAR TRACERS OF TURBULENT SHOCKS IN GIANT MOLECULAR CLOUDS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Molecular cloud; Turbulence; Physics; Supersonic speed; Shock (circulatory); Ambipolar diffusion; Dissipation; Astrophysics; Magnetohydrodynamic turbulence; Radiative cooling; Radiative transfer; Shock wave; Computational physics; Mechanics; Atomic physics; Magnetohydrodynamics; Plasma; Thermodynamics; Nuclear physics; Optics","score_opus":0.008041444184798104,"score_gpt":0.2365558549570359,"score_spread":0.2285144107722378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006321533","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978886,0.000041203508,0.0012560766,0.000031459782,0.000004246305,0.000009131687,0.00007590203,0.00008688121,0.0006065041],"genre_scores_gemma":[0.9989666,0.000028767623,0.00073257013,0.000011627417,0.0000027151768,0.0000053845365,0.00010897035,0.000020950478,0.00012240725],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99991286,0.000019432908,0.0000047404983,0.000014804164,0.000018117918,0.00003006431],"domain_scores_gemma":[0.9997106,0.00009971985,0.00006353709,0.000026776648,0.00002787692,0.00007150852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002596878,0.00040870122,0.00034965354,0.00047245368,0.0004739806,0.0008759993,0.0004822203,0.00043506717,0.0007275899],"category_scores_gemma":[0.0010526036,0.00038150095,0.0003905916,0.00059763656,0.00052930287,0.00049648725,0.0006079444,0.00044536486,0.000080369704],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080576283,0.00027364105,0.07316487,0.000055798413,0.00016032004,0.000358174,0.00045915053,0.84477186,0.065991424,0.0089448,0.00043208385,0.004582177],"study_design_scores_gemma":[0.00018163989,0.00015394598,0.029217122,0.000010444721,0.000039159022,0.00005284076,0.000111356916,0.95506877,0.0125519065,0.0020076302,0.00057530485,0.000029819095],"about_ca_topic_score_codex":0.008587881,"about_ca_topic_score_gemma":0.0061454587,"teacher_disagreement_score":0.008587881,"about_ca_system_score_codex":0.0011444603,"about_ca_system_score_gemma":0.00032945722,"threshold_uncertainty_score":0.017075777},"labels":[],"label_agreement":null},{"id":"W2006331538","doi":"10.1088/0004-637x/720/1/872","title":"A DETAILED SPECTROPOLARIMETRIC ANALYSIS OF THE PLANET-HOSTING STAR WASP-12<sup>,</sup>","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Planet; Physics; Exoplanet; Astrophysics; Astronomy; Stars; Stellar magnetic field; Photosphere; Stellar atmosphere; Planetary system; Giant planet; Spectral line; Magnetic field; Coronal mass ejection","score_opus":0.008064519357257872,"score_gpt":0.21456821211058758,"score_spread":0.2065036927533297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006331538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9602807,0.00084350863,0.016159125,0.00018896219,0.000075642594,0.000065299726,0.0098346695,0.00055126,0.012000858],"genre_scores_gemma":[0.9626156,0.00039615767,0.02299342,0.000074507196,0.00005506673,0.000025658153,0.011052114,0.00011386144,0.0026735787],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999362,0.00000474088,0.0000040715586,0.00002556339,0.000020899439,0.000008542077],"domain_scores_gemma":[0.99979764,0.000017416742,0.000034672623,0.000035781097,0.00008642184,0.000028133212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010854163,0.00027628193,0.00017492038,0.0010320442,0.00029714656,0.00036054003,0.00015212293,0.00021259404,0.0023116472],"category_scores_gemma":[0.00019249547,0.00009659588,0.0002406268,0.00082687475,0.00013429894,0.0002714153,0.00029423222,0.00019620136,0.0011095041],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026350247,0.000033851473,0.31691182,0.00014127263,0.00009210388,0.00029582134,0.00012583876,0.0006639174,0.6196433,0.0003362886,0.0019214185,0.05957087],"study_design_scores_gemma":[0.0000051288202,0.000081422455,0.8827273,0.000012517059,0.000059643495,0.000786403,0.00027064956,0.002335176,0.100584336,0.00031732282,0.012808011,0.000012149664],"about_ca_topic_score_codex":0.00097645586,"about_ca_topic_score_gemma":0.0021233915,"teacher_disagreement_score":0.0023116472,"about_ca_system_score_codex":0.00017402934,"about_ca_system_score_gemma":0.00008658969,"threshold_uncertainty_score":0.007733226},"labels":[],"label_agreement":null},{"id":"W2006417131","doi":"10.1086/529421","title":"A Search for Dark Matter Annihilation with the Whipple 10 m Telescope","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; WIMP; Astrophysics; Dark matter; Weakly interacting massive particles; Astronomy; Galaxy; Globular cluster; Annihilation; Luminosity; Particle physics; Scalar field dark matter; Cosmology; Dark energy","score_opus":0.012402916211791485,"score_gpt":0.2303047631868583,"score_spread":0.21790184697506682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006417131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98240525,0.0016405273,0.005008106,0.00050489185,0.000032036933,0.00007543244,0.0011559956,0.00033697038,0.008840719],"genre_scores_gemma":[0.9824692,0.0005997782,0.012582327,0.00023859534,0.00006847968,0.000035280216,0.0021074344,0.000025339246,0.0018735504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976045,0.000030050385,0.0000058708365,0.00008014781,0.000073151976,0.000050302417],"domain_scores_gemma":[0.9993019,0.00011195726,0.0002651531,0.0000684522,0.000046323657,0.00020620607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000790227,0.00047052288,0.00029862137,0.0016500768,0.0005771349,0.0005298609,0.00044243544,0.0005352642,0.0014321669],"category_scores_gemma":[0.0005386909,0.0002937504,0.0003323618,0.0011374213,0.00028218632,0.0004955449,0.00096181245,0.00047077413,0.0004361242],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008019322,0.0002669257,0.7252746,0.00023168534,0.0003922147,0.0048135165,0.0013956899,0.0026439936,0.13226895,0.0116906,0.011686292,0.10853358],"study_design_scores_gemma":[0.00015519901,0.00068477046,0.9316842,0.00011695323,0.00019257262,0.0038534696,0.00036841328,0.011548121,0.015171644,0.0047182995,0.03142796,0.00007844907],"about_ca_topic_score_codex":0.0019768106,"about_ca_topic_score_gemma":0.0059185214,"teacher_disagreement_score":0.0019768106,"about_ca_system_score_codex":0.00053632347,"about_ca_system_score_gemma":0.0003997009,"threshold_uncertainty_score":0.0047911406},"labels":[],"label_agreement":null},{"id":"W2006443965","doi":"10.1088/0004-637x/702/2/1593","title":"FOLLOW-UP STUDIES OF THE PULSATING MAGNETIC WHITE DWARF SDSS J142625.71+575218.3","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"Photometry (optics); White dwarf; Luminosity; Binary number; Radial velocity; Orbital motion; Asteroseismology; Oscillation (cell signaling)","score_opus":0.021137079743946918,"score_gpt":0.2590631547678916,"score_spread":0.2379260750239447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006443965","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99591404,0.0002825969,0.00022089457,0.00005618082,0.000012634123,0.00002146656,0.0005712454,0.000016378734,0.0029047052],"genre_scores_gemma":[0.99157834,0.0001826066,0.0009959905,0.00008993231,0.000024551897,0.000020190677,0.0027632122,0.000018890305,0.0043263123],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984694,0.0000077216155,0.0000057086013,0.000041123847,0.000042429423,0.000056057495],"domain_scores_gemma":[0.99949396,0.000027137838,0.00013586828,0.000035715788,0.00012329782,0.00018398254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002627396,0.00031401648,0.0003997872,0.0017649301,0.00096745184,0.00040823242,0.00024936182,0.00022087745,0.0018582826],"category_scores_gemma":[0.00034528776,0.00011589315,0.0002797244,0.0009477211,0.00020011114,0.00021468275,0.00047512932,0.00028054832,0.0006109398],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006303381,0.00039855263,0.7638103,0.00017219572,0.00015706332,0.0021044288,0.0016785741,0.0005441877,0.19459541,0.00088564877,0.0029176464,0.0321057],"study_design_scores_gemma":[0.000011938336,0.00015406254,0.98702115,0.000007585799,0.000032383996,0.00027360802,0.00024708526,0.00018442722,0.0048531727,0.00009667771,0.0071086283,0.000009262768],"about_ca_topic_score_codex":0.008717959,"about_ca_topic_score_gemma":0.023263233,"teacher_disagreement_score":0.008717959,"about_ca_system_score_codex":0.00045485736,"about_ca_system_score_gemma":0.00021786534,"threshold_uncertainty_score":0.017334402},"labels":[],"label_agreement":null},{"id":"W2006468976","doi":"10.1088/0004-637x/714/1/571","title":"THE JAMES CLERK MAXWELL TELESCOPE NEARBY GALAXIES LEGACY SURVEY. II. WARM MOLECULAR GAS AND STAR FORMATION IN THREE FIELD SPIRAL GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; National Research Council Canada; McMaster University; Queen's University; Royal Military College of Canada; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; James Clerk Maxwell Telescope; Galaxy; Spiral galaxy; Star formation; Luminous infrared galaxy; Telescope; Astronomy","score_opus":0.007403883549276288,"score_gpt":0.21154702608431059,"score_spread":0.2041431425350343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006468976","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9801672,0.0002526808,0.0001663905,0.0001243408,0.00000710784,0.000031400523,0.01491515,0.000025626405,0.0043100705],"genre_scores_gemma":[0.9666307,0.0003699672,0.0011047497,0.00014465081,0.000028895667,0.000050681032,0.026404103,0.000019386482,0.005246778],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982303,0.000016039587,0.000013702648,0.000052985764,0.00004457617,0.000049648082],"domain_scores_gemma":[0.999106,0.0000413215,0.0002705361,0.0001332214,0.00011721158,0.00033181472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040209503,0.00018115916,0.00017841533,0.0020544396,0.0005330518,0.0004598189,0.00032817633,0.00019453619,0.0023964948],"category_scores_gemma":[0.00051711226,0.00015055276,0.00018087332,0.0013331725,0.00022046652,0.0003597903,0.0005960114,0.00021915852,0.0008985594],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000074719595,0.00003345353,0.9895918,0.000015169915,0.000028299164,0.00005700566,0.000250762,0.000042314277,0.0017453276,0.00013470501,0.0021219042,0.0059046065],"study_design_scores_gemma":[0.000004891284,0.000009090878,0.998089,0.0000021816588,0.0000058423543,0.000025321653,0.000055914923,0.000025640276,0.000080628444,0.000011751788,0.0016879413,0.0000016712497],"about_ca_topic_score_codex":0.12320284,"about_ca_topic_score_gemma":0.33897024,"teacher_disagreement_score":0.12320284,"about_ca_system_score_codex":0.0009296191,"about_ca_system_score_gemma":0.00045923982,"threshold_uncertainty_score":0.2449714},"labels":[],"label_agreement":null},{"id":"W2006486406","doi":"10.1086/428037","title":"Hot Jupiters and Hot Spots: The Short‐ and Long‐Term Chromospheric Activity on Stars with Giant Planets","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":283,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Hot Jupiter; Physics; Stars; Astrophysics; Planet; Jupiter (rocket family); Astronomy; K-type main-sequence star; RADIUS; T Tauri star; Exoplanet","score_opus":0.00930199675316888,"score_gpt":0.21271123109056375,"score_spread":0.20340923433739488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006486406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99959105,0.000112074384,0.000022542685,0.0000050375525,7.530347e-7,0.0000014611819,0.000082529936,0.0000011814652,0.0001834275],"genre_scores_gemma":[0.99961036,0.00004305334,0.000044754215,0.000005761709,0.000004667145,0.0000019206,0.00018173612,0.0000011223334,0.00010661577],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998411,0.000027905004,0.000014975181,0.000041663912,0.00003292695,0.000041340507],"domain_scores_gemma":[0.99921274,0.00010964683,0.00036247296,0.000048662492,0.00006743263,0.00019900958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023543756,0.00013656166,0.00016539787,0.00070636626,0.00024920946,0.0003986609,0.00016335564,0.00025157531,0.0007321987],"category_scores_gemma":[0.000744963,0.00008221616,0.00014510915,0.00069261,0.0003036515,0.00032120495,0.0004071782,0.00017786432,0.00011057395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103887054,0.000014895665,0.9919367,0.00001164315,0.000027975224,0.00008348833,0.00020571776,0.00004593608,0.004465313,0.000015698875,0.000037754005,0.0030510162],"study_design_scores_gemma":[7.358607e-7,0.000022957454,0.9995622,0.0000010829311,0.000004969412,0.000082508195,0.00004832252,0.000023833303,0.00017441351,0.0000054214556,0.00007234711,0.0000010892359],"about_ca_topic_score_codex":0.0032201724,"about_ca_topic_score_gemma":0.007170877,"teacher_disagreement_score":0.0032201724,"about_ca_system_score_codex":0.00023606222,"about_ca_system_score_gemma":0.00010788494,"threshold_uncertainty_score":0.00640285},"labels":[],"label_agreement":null},{"id":"W2006641223","doi":"10.1086/308523","title":"Magnetic Fields in Star‐forming Molecular Clouds. I. The First Polarimetry of OMC‐3 in Orion A","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"James Clerk Maxwell Telescope; Protein filament; Physics; Astrophysics; Polarization (electrochemistry); Outflow; Polarimeter; Polarimetry; Sky; Serpens; Molecular cloud; Magnetic field; Star formation; Radiative transfer; Jovian; Astronomy; Stars; Planet; Optics; Scattering; Materials science; Chemistry; Meteorology","score_opus":0.005149072101802119,"score_gpt":0.21599662594869246,"score_spread":0.21084755384689033,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006641223","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959099,0.00052648317,0.00029929125,0.00006841407,0.000010890729,0.0000157143,0.00054495496,0.000036593578,0.0025877287],"genre_scores_gemma":[0.99845827,0.00012117055,0.00061100186,0.000025054966,0.000024133737,0.0000055645187,0.00050571,0.0000072208964,0.00024186859],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999039,0.000007889153,0.000003652619,0.00002428705,0.00003073481,0.000029424575],"domain_scores_gemma":[0.9996087,0.00004129768,0.00014971681,0.000028909395,0.0000931766,0.000078304234],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019304908,0.00024325999,0.00019882942,0.0010719702,0.00066558435,0.0006306977,0.0003005467,0.00038777618,0.0006948661],"category_scores_gemma":[0.0004956744,0.00017035432,0.00015330315,0.0008018161,0.00040315514,0.00025838133,0.00047215604,0.00046326526,0.00022085701],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005817675,0.00009452474,0.7375552,0.00017487114,0.00007364305,0.0010671349,0.0012594227,0.0009091323,0.22522156,0.0005827101,0.00097632816,0.031503726],"study_design_scores_gemma":[0.00001397265,0.000045842044,0.9934962,0.000017351624,0.000013637003,0.00017715171,0.00008905105,0.0004546932,0.0036430988,0.00010540478,0.0019379403,0.0000055904216],"about_ca_topic_score_codex":0.012908285,"about_ca_topic_score_gemma":0.012193818,"teacher_disagreement_score":0.012908285,"about_ca_system_score_codex":0.0006402606,"about_ca_system_score_gemma":0.0002442007,"threshold_uncertainty_score":0.025666296},"labels":[],"label_agreement":null},{"id":"W2006687150","doi":"10.1088/0004-637x/799/2/180","title":"A STATISTICAL RECONSTRUCTION OF THE PLANET POPULATION AROUND<i>KEPLER</i>SOLAR-TYPE STARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomical and nuclear sciences","field":"Physics and Astronomy","cited_by":168,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Kepler; Planet; Stars; Astrobiology; Astronomy; Population; Physics; Astrophysics; Sociology; Demography","score_opus":0.014843387156913489,"score_gpt":0.22835146325264583,"score_spread":0.21350807609573233,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006687150","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.990281,0.000053127726,0.005963595,0.000052270298,0.0000024594583,0.0000068465956,0.002413833,0.00026024622,0.0009665677],"genre_scores_gemma":[0.9921301,0.00004612407,0.0030121221,0.000013538265,0.000007868032,0.000009160011,0.004502605,0.000031610674,0.0002468779],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997918,0.000036272955,0.000012994348,0.000087804794,0.000035760047,0.000035363893],"domain_scores_gemma":[0.9973447,0.00080419664,0.00074238976,0.00047528037,0.00039827728,0.00023519738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005534487,0.00022881408,0.00017558946,0.0022006815,0.00026800536,0.0005051808,0.00040054042,0.00034744813,0.0012886813],"category_scores_gemma":[0.003843285,0.00025376462,0.00045956846,0.0018741346,0.00029200467,0.00048475736,0.00045231864,0.00035762464,0.00078777934],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015047567,0.000041547923,0.94020367,0.000025742687,0.00011284292,0.00010732669,0.00017286096,0.032611676,0.004671036,0.0015692506,0.0014370152,0.018896647],"study_design_scores_gemma":[0.0000106724365,0.000055845598,0.87762177,0.000007915485,0.000026273541,0.00033442458,0.0001360815,0.11719906,0.0016251052,0.0010009751,0.0019547485,0.00002717397],"about_ca_topic_score_codex":0.008987514,"about_ca_topic_score_gemma":0.0063684476,"teacher_disagreement_score":0.008987514,"about_ca_system_score_codex":0.00035857456,"about_ca_system_score_gemma":0.0003264305,"threshold_uncertainty_score":0.017870426},"labels":[],"label_agreement":null},{"id":"W2006707139","doi":"10.1086/587615","title":"Radial and Nonradial Oscillation Modes in Rapidly Rotating Stars","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Eigenfunction; Spherical harmonics; Physics; Perturbation (astronomy); Harmonics; Rotation (mathematics); Oscillation (cell signaling); Stars; Angular velocity; Classical mechanics; Wavenumber; Mechanics; Astrophysics; Eigenvalues and eigenvectors; Optics; Geometry; Mathematics; Quantum mechanics","score_opus":0.014243941775616147,"score_gpt":0.2212372096128741,"score_spread":0.20699326783725797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006707139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96898186,0.00020659823,0.028671086,0.0000693879,0.000014110834,0.000014115571,0.000044290842,0.00012431355,0.001874129],"genre_scores_gemma":[0.992224,0.00008980525,0.0070494674,0.000011958845,0.00000565739,0.00001247331,0.00005770081,0.00003232481,0.000516628],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999124,0.000023292807,0.000006379752,0.000016062297,0.000026467458,0.000015390848],"domain_scores_gemma":[0.9997259,0.00008977848,0.00007489306,0.000040279665,0.000040796505,0.000028503566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028908259,0.0003608108,0.00032385948,0.00028315163,0.0002571638,0.00041220177,0.00041908523,0.00044235383,0.00047840286],"category_scores_gemma":[0.0010008309,0.0003291615,0.00045734187,0.00023134405,0.0004011482,0.00045376082,0.00046339314,0.00035670956,0.00017289899],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001481905,0.000087437984,0.015628353,0.00008576167,0.000033441953,0.00031307657,0.00023939043,0.86305004,0.100155346,0.00833158,0.00018420354,0.011743132],"study_design_scores_gemma":[0.000017111492,0.000056282734,0.0038624522,0.0000046256905,0.0000046478804,0.0000667572,0.000022424843,0.98480564,0.00911081,0.0018123143,0.00022564403,0.000011396885],"about_ca_topic_score_codex":0.0018251264,"about_ca_topic_score_gemma":0.00083314575,"teacher_disagreement_score":0.0018251264,"about_ca_system_score_codex":0.0003744153,"about_ca_system_score_gemma":0.0002754637,"threshold_uncertainty_score":0.0036290884},"labels":[],"label_agreement":null},{"id":"W2006720372","doi":"10.1088/0004-637x/765/1/17","title":"ON THE INTRINSIC CONTINUUM LINEAR POLARIZATION OF CLASSICAL BE STARS DURING DISK GROWTH AND DISSIPATION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Stars; Dissipation; Polarization (electrochemistry); Polarimetry; Scattering; Stokes parameters; Linear polarization","score_opus":0.007265945752109227,"score_gpt":0.2129336994554615,"score_spread":0.20566775370335227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006720372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99726224,0.000024866747,0.0020404952,0.000015714702,9.592559e-7,0.00000270319,0.000051947594,0.000020458303,0.00058066996],"genre_scores_gemma":[0.99931884,0.000025175043,0.00046894333,0.0000034191019,0.0000014178861,0.0000020550515,0.00008836205,0.0000074010745,0.00008444369],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999403,0.000013272641,0.0000020387436,0.000017330576,0.000012825943,0.00001420786],"domain_scores_gemma":[0.99941313,0.0002952641,0.0001227489,0.000048505575,0.00006137072,0.000059015205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029351885,0.00023098942,0.00017851352,0.00051598425,0.00028201123,0.00039696135,0.00024218317,0.00019721698,0.0005318697],"category_scores_gemma":[0.001199469,0.00015857935,0.00020206122,0.0004350834,0.00042091453,0.00030039632,0.00028305312,0.0003142318,0.000100203506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008550818,0.00033045927,0.5072676,0.00009133689,0.00013883742,0.000999657,0.00089588173,0.31741065,0.14236976,0.0058585145,0.00040883906,0.023373358],"study_design_scores_gemma":[0.000027635742,0.00012532625,0.34146234,0.000009188308,0.00002378273,0.000236982,0.0001582113,0.6325307,0.023147453,0.001959023,0.0002867395,0.000032638414],"about_ca_topic_score_codex":0.0017009767,"about_ca_topic_score_gemma":0.0012847418,"teacher_disagreement_score":0.0017009767,"about_ca_system_score_codex":0.0002717123,"about_ca_system_score_gemma":0.00011487201,"threshold_uncertainty_score":0.003382206},"labels":[],"label_agreement":null},{"id":"W2006803551","doi":"10.1088/0004-637x/758/1/23","title":"RESOLVING THE RADIO SOURCE BACKGROUND: DEEPER UNDERSTANDING THROUGH CONFUSION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":229,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Jansky; Galaxy; Source counts; Astronomy; Confusion; Surface brightness; Bulge; Radio galaxy; Redshift","score_opus":0.043416742690431144,"score_gpt":0.2568121655870615,"score_spread":0.21339542289663035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006803551","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9022217,0.0017850236,0.08947581,0.0005080364,0.000020785219,0.000028441636,0.00028478345,0.00031772707,0.0053577474],"genre_scores_gemma":[0.9803515,0.00050408393,0.018153382,0.000112482325,0.000042914566,0.000014205686,0.00024446912,0.00005558559,0.00052130286],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996618,0.00005954049,0.000022912516,0.000088924455,0.00008452965,0.000082323524],"domain_scores_gemma":[0.99849594,0.000598791,0.00036258102,0.00017238232,0.000232667,0.00013761407],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009252196,0.0005182163,0.00044342215,0.0020334348,0.0005470951,0.0031102414,0.00089451985,0.00047272735,0.00093746645],"category_scores_gemma":[0.0037805983,0.00042849203,0.00027994823,0.00088117784,0.0007466246,0.0035288217,0.002514228,0.0007679723,0.00026661486],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006546064,0.00016183419,0.43372175,0.00047643934,0.00015306831,0.0015872824,0.0076963985,0.023095476,0.1672295,0.033528633,0.001231105,0.33046392],"study_design_scores_gemma":[0.00005066846,0.00020461067,0.63870275,0.00018088783,0.0001376676,0.0016909626,0.0025904994,0.21304159,0.05868195,0.07064344,0.013851631,0.00022339946],"about_ca_topic_score_codex":0.0033471545,"about_ca_topic_score_gemma":0.004046396,"teacher_disagreement_score":0.0033471545,"about_ca_system_score_codex":0.0008883923,"about_ca_system_score_gemma":0.0003830801,"threshold_uncertainty_score":0.0066553354},"labels":[],"label_agreement":null},{"id":"W2006847916","doi":"10.1086/422465","title":"Quantitative Analysis of the Oscillation Spectrum of η Bootis","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced NMR Techniques and Applications","field":"Chemistry","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Metallicity; Physics; Oscillation (cell signaling); Bumping; Astrophysics; Adiabatic process; Luminosity; Spectral line; Mode (computer interface); Stars; Computational physics; Astronomy; Galaxy; Condensed matter physics; Thermodynamics","score_opus":0.013312161877180304,"score_gpt":0.288639446169005,"score_spread":0.2753272842918247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006847916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99302894,0.00006329411,0.005622166,0.000016765129,0.0000022289278,0.000004005556,0.0003251445,0.000059679278,0.0008778207],"genre_scores_gemma":[0.9980269,0.000022508697,0.0014554401,0.0000022250822,0.0000019598283,0.0000037746436,0.00035789094,0.0000143022835,0.00011503629],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999299,0.00000890587,0.0000025979573,0.000028403869,0.000017262915,0.000012908665],"domain_scores_gemma":[0.9995844,0.00015021543,0.00009367291,0.00005133831,0.000075503674,0.00004481772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029035372,0.00019059551,0.00014258132,0.00082739216,0.00019455531,0.0002684895,0.00021333907,0.00013864935,0.0009942879],"category_scores_gemma":[0.0012485671,0.00013698658,0.00017040565,0.00040574255,0.00026118386,0.00028604842,0.0002506024,0.00014003395,0.0001206386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005601195,0.000046219822,0.5033491,0.00021555295,0.00016306191,0.00039355113,0.0007920804,0.06639685,0.37280637,0.0070782355,0.0005250877,0.04767372],"study_design_scores_gemma":[0.000020376187,0.000086966626,0.8195239,0.00001674254,0.00005007508,0.0002473301,0.00020081233,0.15430726,0.020129744,0.003588236,0.001794533,0.000033980967],"about_ca_topic_score_codex":0.0023490933,"about_ca_topic_score_gemma":0.002373177,"teacher_disagreement_score":0.0023490933,"about_ca_system_score_codex":0.00027880844,"about_ca_system_score_gemma":0.00007253304,"threshold_uncertainty_score":0.004670799},"labels":[],"label_agreement":null},{"id":"W2006860162","doi":"10.1088/0004-637x/788/2/181","title":"USING GAPS IN<i>N</i>-BODY TIDAL STREAMS TO PROBE MISSING SATELLITES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Halo; Dark matter; Milky Way; STREAMS; Dark matter halo; Spectral line; Astronomy; Stars; Galaxy","score_opus":0.010669338019575125,"score_gpt":0.23700224119659657,"score_spread":0.22633290317702145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006860162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99464154,0.000026656684,0.003621456,0.00007374402,0.000008203272,0.000012776058,0.00029461228,0.00012364377,0.0011974832],"genre_scores_gemma":[0.99618894,0.000021629114,0.0031470116,0.0000224353,0.0000046874934,0.000013200308,0.0003585616,0.000026670974,0.00021699994],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992335,0.00002010674,0.0000034258978,0.000018470313,0.000014131837,0.000020416132],"domain_scores_gemma":[0.99920815,0.00039864585,0.00014603004,0.000058901285,0.00006368293,0.0001245564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037666768,0.0003263698,0.00025006084,0.00038524045,0.00036703402,0.0004999295,0.0006646338,0.0005679546,0.0008639037],"category_scores_gemma":[0.0021048938,0.00021696794,0.00032488373,0.00047072166,0.00044559015,0.00050771085,0.0004559357,0.00046585893,0.000098988254],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016587539,0.00009526275,0.03580542,0.000020224144,0.00005582053,0.00013605789,0.000083648905,0.95770705,0.0015641204,0.001844018,0.00037436537,0.0021480594],"study_design_scores_gemma":[0.000027665845,0.000028580527,0.003209169,0.0000025846825,0.0000053976732,0.000011121591,0.000028658667,0.995353,0.00045794874,0.0007416786,0.0001288962,0.0000053133112],"about_ca_topic_score_codex":0.019087687,"about_ca_topic_score_gemma":0.015010467,"teacher_disagreement_score":0.019087687,"about_ca_system_score_codex":0.0006191042,"about_ca_system_score_gemma":0.00046207447,"threshold_uncertainty_score":0.03795314},"labels":[],"label_agreement":null},{"id":"W2006959568","doi":"10.1088/0004-637x/761/2/115","title":"THE 217.5 nm BAND, INFRARED ABSORPTION, AND INFRARED EMISSION FEATURES IN HYDROGENATED AMORPHOUS CARBON NANOPARTICLES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Amorphous carbon; Carbon fibers; Infrared; Infrared spectroscopy; Cosmic dust; Spectral line; Analytical Chemistry (journal); Naphthalene; Silicate","score_opus":0.006484026191912903,"score_gpt":0.22122737859508423,"score_spread":0.21474335240317133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2006959568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965591,0.00032949532,0.0015723149,0.00001877813,0.0000061458277,0.0000064979026,0.000049799415,0.000016696806,0.0014411788],"genre_scores_gemma":[0.9975006,0.00013093588,0.0015167522,0.000012672002,0.0000030243082,0.0000073488627,0.00010084447,0.000011740448,0.0007161744],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993217,0.0000066841935,0.0000035840474,0.000017732891,0.000030266036,0.000009513563],"domain_scores_gemma":[0.99993515,0.000017638895,0.000016442795,0.000008824525,0.000013582944,0.00000830589],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008221279,0.00010829155,0.000060624403,0.0001687084,0.00014115566,0.0001285692,0.00012362152,0.00015038504,0.00028257509],"category_scores_gemma":[0.0001169693,0.00008416658,0.000108082124,0.00009664167,0.00017572429,0.00009778652,0.00008490968,0.00015125221,0.000103402424],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000014377559,0.0000067782844,0.00019704932,0.000017580878,0.0000027792114,0.000024675988,0.000012799732,0.00011242467,0.9986299,0.00007621463,0.000017659771,0.0008878283],"study_design_scores_gemma":[0.0000025500324,0.000046908473,0.0030896813,0.0000016559059,0.0000042508223,0.000047553658,0.000011111635,0.000590242,0.99571735,0.000028403116,0.00045831982,0.0000020694956],"about_ca_topic_score_codex":0.00039087655,"about_ca_topic_score_gemma":0.00083632336,"teacher_disagreement_score":0.00039087655,"about_ca_system_score_codex":0.0001629552,"about_ca_system_score_gemma":0.000054544318,"threshold_uncertainty_score":0.0011823773},"labels":[],"label_agreement":null},{"id":"W2007012087","doi":"10.1086/510150","title":"Current Star Formation in the Perseus Molecular Cloud: Constraints from Unbiased Submillimeter and Mid‐Infrared Surveys","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Young stellar object; Physics; Astrophysics; Star formation; James Clerk Maxwell Telescope; Molecular cloud; Serpens; Infrared; Astronomy; Extinction (optical mineralogy); Galaxy; Stars; Optics","score_opus":0.01563834599074291,"score_gpt":0.25291917100380706,"score_spread":0.23728082501306416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007012087","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991904,0.000055169785,0.00011388008,0.000007024735,5.512135e-7,0.0000021876956,0.00033024623,0.0000037767525,0.00029671617],"genre_scores_gemma":[0.99872595,0.00007802958,0.00020977628,0.000010930068,0.000004352916,0.0000048353454,0.0008581225,0.0000022476452,0.000105627696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984634,0.00002152164,0.000011596046,0.000046480047,0.000039138708,0.000034980476],"domain_scores_gemma":[0.9991653,0.00016721476,0.0002966598,0.000118089345,0.000112334536,0.00014037399],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023777828,0.00021527759,0.00018078074,0.0012306349,0.000253132,0.000511369,0.00025647748,0.00013323885,0.0008201485],"category_scores_gemma":[0.0014255198,0.00012649666,0.00011711819,0.000811325,0.00024770948,0.0003306022,0.00057682034,0.00011271211,0.00028691508],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000016789807,0.0000052450087,0.995357,0.000002984335,0.000011638248,0.000039649385,0.00009252448,0.00015690313,0.0013824902,0.0000501133,0.00006949956,0.0028150585],"study_design_scores_gemma":[0.0000015653366,0.000008033734,0.9987649,0.0000019550591,0.000004399013,0.00005343346,0.000089613255,0.0004876623,0.00032662207,0.00003759356,0.00022258658,0.0000016298656],"about_ca_topic_score_codex":0.01144831,"about_ca_topic_score_gemma":0.020482881,"teacher_disagreement_score":0.01144831,"about_ca_system_score_codex":0.00020612273,"about_ca_system_score_gemma":0.00016973043,"threshold_uncertainty_score":0.022763371},"labels":[],"label_agreement":null},{"id":"W2007098366","doi":"10.1086/312743","title":"Measurement of a Peak in the Cosmic Microwave Background Power Spectrum from the North American Test Flight of Boomerang","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cosmic microwave background; Angular resolution (graph drawing); Bolometer; Cosmic infrared background; Spectral density; Amplitude; Telescope; Microwave","score_opus":0.008877109989786873,"score_gpt":0.22247521078771207,"score_spread":0.21359810079792518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007098366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996644,0.000054285792,0.0007048676,0.00005437206,0.0000064616493,0.000009434895,0.00028373874,0.000056783534,0.002186121],"genre_scores_gemma":[0.9979036,0.000042379274,0.00094174506,0.000029242297,0.000009449973,0.000008528152,0.00060660194,0.000019429921,0.00043906996],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990594,0.000011788372,0.0000014557064,0.000024851837,0.000029964833,0.000026004198],"domain_scores_gemma":[0.9998097,0.000019395133,0.000032715794,0.000022502783,0.00005023222,0.00006565482],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014856312,0.0003128168,0.000156208,0.00047830705,0.0006037304,0.00027984096,0.00017978852,0.00017865794,0.00068924495],"category_scores_gemma":[0.00027232256,0.00014953781,0.00010645841,0.00040329696,0.00032067744,0.00019757553,0.00038525258,0.0004308437,0.00015362127],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017829639,0.00035557567,0.5888084,0.00009137505,0.00028908154,0.0010438679,0.0020934946,0.0018934227,0.34768805,0.0011186056,0.0035172545,0.051317975],"study_design_scores_gemma":[0.000020129446,0.000116679366,0.9868814,0.0000034940724,0.000029251158,0.0001780611,0.000080774276,0.0010021131,0.009232339,0.000076379554,0.0023654439,0.000013817268],"about_ca_topic_score_codex":0.013886809,"about_ca_topic_score_gemma":0.0413319,"teacher_disagreement_score":0.013886809,"about_ca_system_score_codex":0.00034521832,"about_ca_system_score_gemma":0.00017338089,"threshold_uncertainty_score":0.02761197},"labels":[],"label_agreement":null},{"id":"W2007111587","doi":"10.1086/592770","title":"Toward Precise Constraints on the Growth of Massive Black Holes","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; QSOS; Eddington luminosity; Physics; Accretion (finance); Luminosity; Luminosity function; Black hole (networking); Astronomy; Quasar; Galaxy","score_opus":0.029004303335403922,"score_gpt":0.23037450689852523,"score_spread":0.2013702035631213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007111587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95783734,0.003649101,0.028876003,0.00035033652,0.000030937812,0.000018881861,0.0007248226,0.00021148448,0.008301138],"genre_scores_gemma":[0.99394315,0.0006051353,0.004630667,0.00006436673,0.000045729812,0.000012379266,0.00042300828,0.000035647103,0.00023983982],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99982786,0.00003856315,0.0000125634815,0.000056877805,0.000033706216,0.000030368],"domain_scores_gemma":[0.9969021,0.0014576613,0.00090397964,0.0002979752,0.00020131173,0.00023695946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001217488,0.00062123913,0.0004341396,0.0011282708,0.00041619546,0.0014349609,0.0007119577,0.00067282846,0.0013765884],"category_scores_gemma":[0.0064759366,0.00054204446,0.00026591597,0.0005172419,0.0006574857,0.0016728968,0.001372751,0.00075383007,0.00051352725],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006110538,0.00008807313,0.65740925,0.0003933857,0.00018270807,0.00070745236,0.00095161994,0.06487202,0.0854072,0.10632577,0.0017157852,0.08133558],"study_design_scores_gemma":[0.00006422526,0.00020306425,0.7437228,0.00020842627,0.00007689587,0.00052917417,0.000630116,0.14107831,0.027642265,0.073073305,0.012666015,0.00010535527],"about_ca_topic_score_codex":0.0008933503,"about_ca_topic_score_gemma":0.0009904668,"teacher_disagreement_score":0.0014349609,"about_ca_system_score_codex":0.0005683082,"about_ca_system_score_gemma":0.00020445252,"threshold_uncertainty_score":0.006438732},"labels":[],"label_agreement":null},{"id":"W2007144646","doi":"10.1088/0004-637x/772/1/59","title":"REPRODUCING THE OBSERVED ABUNDANCES IN RCB AND HdC STARS WITH POST-DOUBLE-DEGENERATE MERGER MODELS—CONSTRAINTS ON MERGER AND POST-MERGER SIMULATIONS AND PHYSICS PROCESSES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Nucleosynthesis; Stars; Envelope (radar); Asymptotic giant branch; Mixing (physics); Stellar evolution; Stellar nucleosynthesis","score_opus":0.02543367429986015,"score_gpt":0.22717600116260397,"score_spread":0.20174232686274382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007144646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99430263,0.00016115682,0.002913682,0.00008934928,0.000011260171,0.000016777492,0.0004527764,0.00008483448,0.0019674944],"genre_scores_gemma":[0.9979265,0.000066487126,0.0011781894,0.00002478124,0.000009613327,0.000016554879,0.00047141666,0.00002502219,0.00028140142],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998839,0.000023568724,0.000007947594,0.00003538827,0.00001643565,0.000032733136],"domain_scores_gemma":[0.99958044,0.00012203392,0.00008725273,0.000069198366,0.000046338115,0.00009473136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003083563,0.0006525814,0.0005881181,0.00029994332,0.00047168508,0.0007606568,0.0010409767,0.000915274,0.0009160518],"category_scores_gemma":[0.0010348216,0.00033054737,0.00081915857,0.00029829782,0.0003739211,0.0006227111,0.0004451726,0.00042874762,0.00020422728],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024199771,0.00016139474,0.04432434,0.00006223823,0.00016981567,0.00024964073,0.00013014546,0.93555677,0.011830599,0.0037300547,0.00032082826,0.00322207],"study_design_scores_gemma":[0.00006345142,0.00005982139,0.011996098,0.0000047057606,0.000033122284,0.00004580637,0.000030735995,0.9849995,0.0013111967,0.0010211556,0.00041853305,0.000015902617],"about_ca_topic_score_codex":0.017402373,"about_ca_topic_score_gemma":0.008488875,"teacher_disagreement_score":0.017402373,"about_ca_system_score_codex":0.0009163486,"about_ca_system_score_gemma":0.0005686171,"threshold_uncertainty_score":0.034602165},"labels":[],"label_agreement":null},{"id":"W2007157556","doi":"10.1086/586694","title":"Evidence for Line‐of‐Sight Structure in a Comparison of X‐Ray and Optical Observations of the High‐Redshift Cluster RCS 043938‐2904.7","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Redshift; Astrophysics; Physics; Cluster (spacecraft); Galaxy cluster; Luminosity; Galaxy; Line-of-sight; Line (geometry); Astronomy; Geometry","score_opus":0.03808920002887188,"score_gpt":0.267182812679761,"score_spread":0.22909361265088912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007157556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937937,0.000106247084,0.00014718529,0.00007177159,0.000005632817,0.0000042484444,0.0007303206,0.000024900555,0.005115874],"genre_scores_gemma":[0.9977197,0.000033732125,0.00027442115,0.00001865183,0.0000036683243,0.000003978664,0.0010500654,0.0000063947314,0.0008892586],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983144,0.000016064505,0.000007946389,0.000059927235,0.000045914774,0.00003861286],"domain_scores_gemma":[0.99913067,0.00009599467,0.0002796402,0.00007870016,0.000245385,0.0001696435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022825277,0.000076364835,0.00011080395,0.0012872221,0.0004855435,0.0005216955,0.0002518424,0.00026664638,0.0038551642],"category_scores_gemma":[0.0008784897,0.00014679477,0.000113003116,0.0011718951,0.00026981387,0.00023260874,0.0006529192,0.0001847932,0.0005672719],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027483245,0.00007285189,0.9360492,0.000042020736,0.0000981613,0.00020427104,0.00093725097,0.00017740946,0.048969567,0.0010371933,0.0017782378,0.010359064],"study_design_scores_gemma":[0.000005167282,0.000008793581,0.9980989,0.000003029778,0.000010796564,0.00005333315,0.00022196073,0.00015013215,0.0003991171,0.000059499755,0.000986957,0.0000022649008],"about_ca_topic_score_codex":0.030583091,"about_ca_topic_score_gemma":0.056988094,"teacher_disagreement_score":0.030583091,"about_ca_system_score_codex":0.00035302222,"about_ca_system_score_gemma":0.00040688677,"threshold_uncertainty_score":0.06081015},"labels":[],"label_agreement":null},{"id":"W2007199658","doi":"10.1088/0004-637x/776/2/87","title":"THE RADIUS DISCREPANCY IN LOW-MASS STARS: SINGLE VERSUS BINARIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":202,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Stars; Physics; Astrophysics; Metallicity; RADIUS; Moment of inertia; Stellar evolution; Rotation (mathematics); Asteroseismology; Stellar rotation; Classical mechanics; Geometry","score_opus":0.011352535218854693,"score_gpt":0.21720865389046343,"score_spread":0.20585611867160875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007199658","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9891844,0.00020641235,0.009337129,0.000022169483,0.0000035487985,0.0000039592164,0.0002547749,0.00011410887,0.0008735799],"genre_scores_gemma":[0.99580294,0.000049829065,0.0037290805,0.0000031423633,0.0000017049788,0.0000037882562,0.00023434877,0.00003597888,0.0001392932],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99979454,0.00005890905,0.000015574356,0.00007723984,0.000036073176,0.000017641933],"domain_scores_gemma":[0.99888927,0.00066149054,0.0001952854,0.000120075376,0.00006517473,0.00006873486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005065,0.00017332453,0.0003967393,0.0005158576,0.00021236471,0.0005916466,0.00056033256,0.00026224056,0.001081179],"category_scores_gemma":[0.0025082189,0.00015137008,0.00022273362,0.0007263702,0.00034630494,0.00053588266,0.0005809236,0.00024599678,0.00026776426],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004272267,0.000055754994,0.41965374,0.00009082724,0.00005945211,0.00022641972,0.00025949767,0.5419381,0.012516511,0.0058493065,0.0003489125,0.018574217],"study_design_scores_gemma":[0.000021346686,0.00008306972,0.117405415,0.000015740134,0.000028502567,0.00031537484,0.000104369494,0.8632294,0.012251763,0.005559039,0.0009569782,0.000029065122],"about_ca_topic_score_codex":0.0036674805,"about_ca_topic_score_gemma":0.0025052347,"teacher_disagreement_score":0.0036674805,"about_ca_system_score_codex":0.00037137445,"about_ca_system_score_gemma":0.00020576615,"threshold_uncertainty_score":0.0072922707},"labels":[],"label_agreement":null},{"id":"W2007217868","doi":"10.1088/0004-637x/734/2/103","title":"CONSTRAINING THE REDSHIFT EVOLUTION OF FIRST RADIO SOURCES IN RCS1 GALAXY CLUSTERS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Galaxy cluster; Redshift; Radio galaxy; Cluster (spacecraft); Brightest cluster galaxy; Galaxy; Galaxy groups and clusters; Sky","score_opus":0.011823859608996637,"score_gpt":0.19872148198144957,"score_spread":0.18689762237245294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007217868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979748,0.00015120719,0.00026692977,0.000059094047,0.0000038102153,0.0000041957796,0.000500437,0.000028563943,0.0010109843],"genre_scores_gemma":[0.9976941,0.00005885243,0.00036596906,0.000011227449,0.0000060491698,0.0000034353945,0.0011538137,0.000013233611,0.00069341017],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976856,0.000025154448,0.000010296875,0.0000814792,0.000039868704,0.00007461985],"domain_scores_gemma":[0.9979988,0.00041403662,0.0005526638,0.00022418251,0.00032261596,0.0004877018],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005069736,0.00018094234,0.0001857606,0.0028778596,0.00058875553,0.0011412231,0.0004399071,0.0004167161,0.00184175],"category_scores_gemma":[0.0025073732,0.00023030023,0.00023787102,0.0014544291,0.00025945096,0.00030760636,0.0008806373,0.0003061123,0.0005708212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007058161,0.00003081207,0.9844887,0.000011542852,0.000038910457,0.000043221,0.0003507976,0.0011979997,0.0036452075,0.0004425334,0.0005399627,0.0091396775],"study_design_scores_gemma":[0.000003227527,0.000008084488,0.99729794,0.0000045683287,0.000012682991,0.000029660518,0.00021732958,0.0013262602,0.0003548542,0.000084218205,0.0006559105,0.0000052348782],"about_ca_topic_score_codex":0.06974158,"about_ca_topic_score_gemma":0.09930038,"teacher_disagreement_score":0.06974158,"about_ca_system_score_codex":0.000871518,"about_ca_system_score_gemma":0.00063420646,"threshold_uncertainty_score":0.13867128},"labels":[],"label_agreement":null},{"id":"W2007359848","doi":"10.1086/510504","title":"Implications of the Cosmic Background Imager Polarization Data","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Polarization (electrochemistry); Spectral density; Spectral line; Astrophysics; Planck; Lambda; COSMIC cancer database; Adiabatic process; Computational physics; Optics; Anisotropy; Astronomy; Quantum mechanics","score_opus":0.020009837729549573,"score_gpt":0.2931758336134066,"score_spread":0.27316599588385704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007359848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9523917,0.00052941224,0.008455104,0.0025645618,0.0001540568,0.000013322521,0.011709859,0.00039357046,0.023788443],"genre_scores_gemma":[0.99387676,0.00016354748,0.0013863526,0.00026769922,0.000079257945,0.0000058853766,0.0034321737,0.00008003956,0.0007082258],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986778,0.0002690737,0.000059897542,0.0003576847,0.00046436465,0.00017108946],"domain_scores_gemma":[0.9935081,0.0030132942,0.0011035724,0.0011227668,0.0009751548,0.00027705505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015607978,0.00043691296,0.00026489847,0.0012116878,0.00040689396,0.0016949904,0.0005385017,0.00036348123,0.0026599776],"category_scores_gemma":[0.006405948,0.00020478497,0.00026643265,0.0027029726,0.00063574786,0.00085366244,0.0007523929,0.00093502447,0.0007020259],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085179775,0.00011376051,0.8892888,0.00008756894,0.00021249187,0.00083044195,0.00030397385,0.0116839055,0.016984686,0.011985126,0.008021395,0.059636123],"study_design_scores_gemma":[0.00003465593,0.00007408461,0.9418844,0.00005303685,0.00012952663,0.0011063135,0.00031492912,0.014019213,0.016201936,0.012323385,0.013798996,0.0000594937],"about_ca_topic_score_codex":0.0056999046,"about_ca_topic_score_gemma":0.0047346205,"teacher_disagreement_score":0.0056999046,"about_ca_system_score_codex":0.0005511992,"about_ca_system_score_gemma":0.00025759471,"threshold_uncertainty_score":0.011333466},"labels":[],"label_agreement":null},{"id":"W2007364201","doi":"10.1086/513102","title":"The Space Motion of the Globular Cluster NGC 6397","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Globular cluster; Proper motion; Milky Way; Photometry (optics); Galaxy; Stellar population; Star cluster; Population; Hubble space telescope","score_opus":0.00479505467118389,"score_gpt":0.20455016702953377,"score_spread":0.1997551123583499,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007364201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99818194,0.00006642618,0.00015240048,0.000022522008,0.0000034061502,0.0000011128354,0.00015068213,0.000023387378,0.0013981434],"genre_scores_gemma":[0.9988249,0.000060863043,0.00029708754,0.0000070426076,0.0000029168466,0.0000018544741,0.00043056716,0.000008279445,0.00036662436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992883,0.0000057212123,0.0000030688873,0.000019331297,0.000030121211,0.000012812274],"domain_scores_gemma":[0.9998293,0.00002551253,0.00004393091,0.000025403086,0.000034255936,0.000041533578],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014805472,0.000092355054,0.00015082907,0.0006160737,0.00038435106,0.00042320383,0.00022077785,0.00018353293,0.0006053094],"category_scores_gemma":[0.0006383422,0.00006726419,0.00010730023,0.0008923928,0.00034577775,0.00014370013,0.00041836154,0.0001681088,0.00030878725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025049536,0.000034429308,0.89315706,0.000040333787,0.00010583584,0.0010272759,0.0013537082,0.018133625,0.040263977,0.0044537717,0.0044669923,0.036712628],"study_design_scores_gemma":[0.000015523603,0.000036082783,0.98014575,0.000011495132,0.000018108853,0.00027180914,0.00023780961,0.01326896,0.0019450767,0.00096116634,0.0030716604,0.000016580465],"about_ca_topic_score_codex":0.032966856,"about_ca_topic_score_gemma":0.027811548,"teacher_disagreement_score":0.032966856,"about_ca_system_score_codex":0.0008988737,"about_ca_system_score_gemma":0.00035000636,"threshold_uncertainty_score":0.06554991},"labels":[],"label_agreement":null},{"id":"W2007365044","doi":"10.1086/377067","title":"The Short Rotation Period of Nereid","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Rotation period; Rotation (mathematics); Albedo (alchemy); Amplitude; Period (music); Light curve; Geometry; Physics; Optics; Astrophysics; Mathematics; History; Art history","score_opus":0.007726946614204695,"score_gpt":0.21530224571849754,"score_spread":0.20757529910429284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007365044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98175645,0.00076151616,0.0022903022,0.00010474089,0.00003999267,0.000022412556,0.0017098733,0.00008581719,0.013228953],"genre_scores_gemma":[0.9966846,0.00013994219,0.00107226,0.000018634595,0.0000097362545,0.0000075768203,0.0013462172,0.000015813028,0.00070515677],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.0000071320464,0.000008632197,0.000058787224,0.000024450437,0.000023229797],"domain_scores_gemma":[0.9996457,0.000042983025,0.00014204507,0.000058295907,0.00005747175,0.000053482785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020323873,0.00018297501,0.0001707477,0.0010141935,0.000409327,0.00040399437,0.00022922264,0.00021202865,0.0015964479],"category_scores_gemma":[0.00075787446,0.00014836833,0.00017941315,0.0008087762,0.00022330093,0.00027222262,0.00046754009,0.00023277203,0.000489529],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007662249,0.00008328647,0.8478706,0.00032862948,0.00014626909,0.0006737621,0.00063481426,0.009333027,0.049901072,0.0035981818,0.004817986,0.08184606],"study_design_scores_gemma":[0.00004616572,0.00014804947,0.92488813,0.00003094204,0.00005298972,0.0006380041,0.00022403357,0.011634609,0.018508894,0.001226429,0.042561453,0.000040221705],"about_ca_topic_score_codex":0.0022100748,"about_ca_topic_score_gemma":0.0035801071,"teacher_disagreement_score":0.0022100748,"about_ca_system_score_codex":0.0006431411,"about_ca_system_score_gemma":0.00023873623,"threshold_uncertainty_score":0.005340636},"labels":[],"label_agreement":null},{"id":"W2007433213","doi":"10.1086/519482","title":"<i>Spitzer</i>Mid‐Infrared Upper Limits on Anomalous X‐Ray Pulsars 1E 1048.1−5937, 1RXS J170849.0−400910, and XTE J1810−197","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Infrared; Astrophysics; Spitzer Space Telescope; Magnetosphere; Flux (metallurgy); Astronomy; Telescope; Magnetic field; Materials science","score_opus":0.010516140750201545,"score_gpt":0.2953841974226726,"score_spread":0.28486805667247106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007433213","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9881799,0.0015358713,0.0018937873,0.00015031658,0.000018910636,0.000008885953,0.00049709936,0.0001480361,0.007567134],"genre_scores_gemma":[0.99550277,0.00058833405,0.001951872,0.00013363898,0.00009740103,0.000019976294,0.0012932615,0.000019324427,0.00039342974],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997514,0.000022433762,0.000018653895,0.00004990694,0.00009428552,0.000063315514],"domain_scores_gemma":[0.99858785,0.0003839452,0.00066039356,0.00012673558,0.00015449681,0.00008650714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055767194,0.0003640151,0.00022332862,0.0020797877,0.00038527293,0.00084002083,0.000556876,0.00041982497,0.0014974389],"category_scores_gemma":[0.0012991212,0.00020912921,0.0001846523,0.00049885723,0.00046250352,0.0005215744,0.0007264228,0.00040289003,0.0005395264],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005928489,0.00013503259,0.83574706,0.00022808589,0.00012386762,0.00064849894,0.00035007924,0.0016220199,0.111531004,0.0038518286,0.003564106,0.041605543],"study_design_scores_gemma":[0.000028137614,0.000083780506,0.9779367,0.00004109105,0.0000660104,0.00070176524,0.000087919696,0.0013582517,0.014498971,0.001302211,0.0038796559,0.00001557598],"about_ca_topic_score_codex":0.00083088037,"about_ca_topic_score_gemma":0.0011042004,"teacher_disagreement_score":0.0020797877,"about_ca_system_score_codex":0.00033509513,"about_ca_system_score_gemma":0.0000728959,"threshold_uncertainty_score":0.0050094724},"labels":[],"label_agreement":null},{"id":"W2007474830","doi":"10.1086/498634","title":"Magnetic Field Generation in Fully Convective Rotating Spheres","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":238,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Equator; Dynamo; Magnetic field; Magnetohydrodynamic drive; Field (mathematics); SPHERES; Convection; Magnetohydrodynamics; Amplitude; Mechanics; Dynamo theory; Classical mechanics; Optics; Latitude; Astronomy","score_opus":0.005149763258343474,"score_gpt":0.21079683512185907,"score_spread":0.20564707186351558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007474830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872247,0.00012155489,0.003986681,0.00031326603,0.00004656599,0.000037420104,0.0003225521,0.00018583616,0.0077614207],"genre_scores_gemma":[0.9978781,0.000058200483,0.0008995087,0.0000388282,0.000014953166,0.000018184843,0.00018890994,0.000032785043,0.0008705509],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998646,0.00002204391,0.0000049677305,0.000017620367,0.00002321483,0.00006744349],"domain_scores_gemma":[0.9996247,0.00007604431,0.000040592717,0.000029669023,0.0000627674,0.00016608795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002281292,0.00050908665,0.0008228665,0.00029956747,0.00078912865,0.0012185983,0.00087970763,0.0008891828,0.002060104],"category_scores_gemma":[0.0012145755,0.00040026786,0.0005271532,0.00038150587,0.001321415,0.00072960067,0.00092980696,0.0005649967,0.00021225134],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040575257,0.00009345766,0.002597095,0.00003297995,0.000038520346,0.00031414977,0.00012128578,0.98212564,0.0070327804,0.0048464285,0.000663379,0.001728615],"study_design_scores_gemma":[0.00022918633,0.00008835052,0.0022804684,0.0000048343923,0.000009816584,0.000035369827,0.00004990167,0.9941204,0.0013214275,0.0014524556,0.0003891841,0.000018656676],"about_ca_topic_score_codex":0.018253317,"about_ca_topic_score_gemma":0.004498721,"teacher_disagreement_score":0.018253317,"about_ca_system_score_codex":0.0012256614,"about_ca_system_score_gemma":0.0011439589,"threshold_uncertainty_score":0.036294162},"labels":[],"label_agreement":null},{"id":"W2007483008","doi":"10.1088/0004-637x/768/2/194","title":"UNDER PRESSURE: STAR CLUSTERS AND THE NEUTRAL HYDROGEN MEDIUM OF TIDAL TAILS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Kinetic energy; Cluster (spacecraft); Star cluster; Star formation; Mean kinetic temperature; Star (game theory); Hydrogen; Radial velocity","score_opus":0.005438788404888204,"score_gpt":0.19252003578675606,"score_spread":0.18708124738186785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007483008","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99896383,0.00016712064,0.00013453145,0.000041791198,0.0000011464681,0.000001203043,0.00006964299,0.0000064710216,0.00061407377],"genre_scores_gemma":[0.9997482,0.0000641166,0.000038782648,0.0000066234606,0.0000025814825,6.4057986e-7,0.000052597872,0.0000012495062,0.00008525013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998934,0.000020890931,0.0000057342727,0.000021691376,0.000019394594,0.000038881946],"domain_scores_gemma":[0.9994924,0.0001042151,0.00018712654,0.00004218625,0.000045106444,0.00012882048],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020251486,0.00012844677,0.00012776247,0.0006525947,0.00040709102,0.0010005564,0.00026526468,0.00023086238,0.0008923524],"category_scores_gemma":[0.0009715141,0.00010989511,0.000080740494,0.00057175773,0.00059694663,0.0009407381,0.00097072066,0.000218333,0.00015318683],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002743872,0.000055277207,0.96759516,0.00004915167,0.000060834973,0.0006608945,0.00096908916,0.002793685,0.011914949,0.00425699,0.00033517808,0.011034359],"study_design_scores_gemma":[0.000015391684,0.00008144196,0.98551196,0.000014933106,0.000023734528,0.000293267,0.0013540725,0.004129347,0.002463831,0.0050180354,0.0010719448,0.000021976908],"about_ca_topic_score_codex":0.0046898997,"about_ca_topic_score_gemma":0.0059915967,"teacher_disagreement_score":0.0046898997,"about_ca_system_score_codex":0.00038582704,"about_ca_system_score_gemma":0.00022703061,"threshold_uncertainty_score":0.009325206},"labels":[],"label_agreement":null},{"id":"W2007517547","doi":"10.1086/367787","title":"The Las Campanas Infrared Survey. IV. The Photometric Redshift Survey and the Rest‐Frame<i>R</i>‐Band Galaxy Luminosity Function at 0.5 ≤ <i>z</i> ≤ 1.5","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Redshift; Luminosity function; Hubble Deep Field; Galaxy; Photometric redshift; Luminosity; Luminous infrared galaxy; Redshift survey","score_opus":0.011283750816137531,"score_gpt":0.21136683796889313,"score_spread":0.2000830871527556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007517547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4638573,0.0061679436,0.0054069054,0.0032178673,0.0004567984,0.0006046548,0.2866755,0.0028873177,0.23072562],"genre_scores_gemma":[0.6995955,0.003416324,0.019608261,0.0021202073,0.00034338122,0.00088519533,0.20975311,0.00037765273,0.063900344],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998072,0.00002006418,0.000007676771,0.00005025092,0.00007475123,0.000040162915],"domain_scores_gemma":[0.9996358,0.000028097931,0.00010815732,0.0000522533,0.00012146697,0.000054163283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036187266,0.00037044892,0.00016564346,0.0027093557,0.0004972033,0.00068302604,0.00066270784,0.0002552312,0.0054284926],"category_scores_gemma":[0.0004811005,0.00015842202,0.00018396779,0.0028529724,0.00020107528,0.0003635173,0.0006004219,0.0006076191,0.002334837],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025194528,0.00021175148,0.39979237,0.00050862756,0.00017481571,0.0003097564,0.00059323147,0.0011348327,0.007456245,0.009933782,0.396082,0.18355061],"study_design_scores_gemma":[0.00003928579,0.000018676745,0.8081998,0.000111638816,0.000031956424,0.00011569972,0.00029270872,0.00060342683,0.0010614373,0.0011198703,0.1883898,0.00001570045],"about_ca_topic_score_codex":0.17459512,"about_ca_topic_score_gemma":0.2108182,"teacher_disagreement_score":0.17459512,"about_ca_system_score_codex":0.0012562171,"about_ca_system_score_gemma":0.0009997464,"threshold_uncertainty_score":0.34715772},"labels":[],"label_agreement":null},{"id":"W2007608095","doi":"10.1088/0004-637x/704/1/324","title":"LESS THAN 10 PERCENT OF STAR FORMATION IN<i>z</i>∼ 0.6 MASSIVE GALAXIES IS TRIGGERED BY MAJOR INTERACTIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics; University of Waterloo","funders":"Science and Technology Facilities Council; Deutsche Forschungsgemeinschaft","keywords":"Physics; Astrophysics; Galaxy; Star formation; Redshift; Stellar mass; COSMIC cancer database; Star (game theory); Cosmic time; Galaxy formation and evolution; Astronomy","score_opus":0.009144016204776884,"score_gpt":0.22761526076723532,"score_spread":0.21847124456245842,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007608095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99424464,0.00038370836,0.0028207786,0.000039951046,0.0000052732635,0.0000056979525,0.00040309087,0.0001542238,0.0019427526],"genre_scores_gemma":[0.9987244,0.00009583976,0.00041329343,0.000015699667,0.000006093163,0.0000028390207,0.000501738,0.0000068654167,0.00023328308],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979705,0.000022543933,0.000011433123,0.00005865005,0.00004989361,0.00006043014],"domain_scores_gemma":[0.99946994,0.000121886915,0.00023209375,0.000084492065,0.00003337425,0.000058264424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027321352,0.00024415064,0.0002675509,0.0005748256,0.0002448285,0.0005323853,0.00031886052,0.0002569974,0.0015270058],"category_scores_gemma":[0.00093929574,0.00016694558,0.00047777756,0.0005122259,0.0003022311,0.00033963693,0.00043933885,0.00014971716,0.00052450906],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012937603,0.000049379294,0.9500317,0.000055906436,0.00018893866,0.00015407628,0.00016022603,0.0030873204,0.018796386,0.0007681757,0.0005772182,0.026001297],"study_design_scores_gemma":[0.000006349439,0.000038194565,0.9893379,0.0000055774176,0.000033109758,0.00019214675,0.000058852078,0.0040581357,0.004414304,0.00045589506,0.0013940181,0.0000054666616],"about_ca_topic_score_codex":0.002363678,"about_ca_topic_score_gemma":0.0029204492,"teacher_disagreement_score":0.002363678,"about_ca_system_score_codex":0.00023094803,"about_ca_system_score_gemma":0.00010451507,"threshold_uncertainty_score":0.0051083565},"labels":[],"label_agreement":null},{"id":"W2007772592","doi":"10.1088/0004-637x/737/2/61","title":"THE ATACAMA COSMOLOGY TELESCOPE: SUNYAEV-ZEL'DOVICH-SELECTED GALAXY CLUSTERS AT 148 GHz IN THE 2008 SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":301,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Office of the Dean for Research, Princeton University; Ministry of Education, Culture, Sports, Science and Technology; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy cluster; South Pole Telescope; Sunyaev–Zel'dovich effect; Redshift; Sky; Cosmology; Cluster (spacecraft); Galaxy; Luminosity; Telescope; Astronomy","score_opus":0.015479369426280101,"score_gpt":0.21800837953926303,"score_spread":0.2025290101129829,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007772592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9664178,0.00045080238,0.00024612856,0.00035937395,0.00004000587,0.00002033357,0.02265209,0.000044978136,0.00976849],"genre_scores_gemma":[0.9702167,0.0002198871,0.00056959526,0.00010630328,0.000024726141,0.000028941056,0.020592064,0.000035028766,0.00820683],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998436,0.000020237063,0.000004873923,0.000041455576,0.000041744075,0.000048081514],"domain_scores_gemma":[0.9996419,0.000033223798,0.00008060447,0.00004034398,0.00008006023,0.00012388435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021907515,0.00009108738,0.0001770815,0.0010566013,0.0004873184,0.0004954167,0.00029046586,0.0001978268,0.003449692],"category_scores_gemma":[0.0006647653,0.00008997271,0.00008281401,0.001289682,0.00017490152,0.0003589193,0.00080698286,0.00028316135,0.0006005273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002159809,0.000042670217,0.94507825,0.00004167723,0.000059519836,0.000099686,0.0010988271,0.0002341539,0.0016464033,0.0017647822,0.030613013,0.01910509],"study_design_scores_gemma":[0.0000058109194,0.0000039864535,0.9878419,0.0000058380815,0.0000044062685,0.000021908565,0.00028281432,0.000095446056,0.00008345016,0.00007103909,0.011581412,0.0000019772092],"about_ca_topic_score_codex":0.097640365,"about_ca_topic_score_gemma":0.24978091,"teacher_disagreement_score":0.097640365,"about_ca_system_score_codex":0.00053618825,"about_ca_system_score_gemma":0.000550081,"threshold_uncertainty_score":0.19414407},"labels":[],"label_agreement":null},{"id":"W2007960515","doi":"10.1088/0004-637x/761/1/35","title":"THE FORMATION OF COSMIC FULLERENES FROM AROPHATIC CLUSTERS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Fullerene Chemistry and Applications","field":"Chemistry","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Fullerene; Planetary nebula; Amorphous carbon; Carbon fibers; Astrobiology; Astrophysics; Amorphous solid; Irradiation; Physics; Materials science; Chemistry; Crystallography; Nuclear physics; Composite material","score_opus":0.012358795566345818,"score_gpt":0.22788662819389602,"score_spread":0.2155278326275502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2007960515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99804616,0.00018804708,0.00024438664,0.000009349242,0.0000035894666,0.0000055040296,0.00008239956,0.0000070643223,0.0014134737],"genre_scores_gemma":[0.99846506,0.00012465489,0.0002657294,0.000014458022,0.0000027887481,0.0000045871466,0.00026240325,0.000006715005,0.000853676],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999175,0.0000048209063,0.0000027327183,0.000023927354,0.0000244838,0.000026531026],"domain_scores_gemma":[0.9999341,0.000011433698,0.000016740989,0.000009073829,0.0000120343375,0.000016689533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006047122,0.00018170306,0.00010002089,0.0002557488,0.00033934967,0.000399211,0.0001293572,0.0003024666,0.00079762976],"category_scores_gemma":[0.00017520548,0.00010545692,0.00010651812,0.0001757853,0.00019998335,0.00026427818,0.00022675845,0.00024570752,0.0001799585],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010201095,0.000016299382,0.0029085253,0.000048231894,0.000013507136,0.00018522018,0.000117075084,0.00064462266,0.9927672,0.0005627067,0.00013470146,0.0024998928],"study_design_scores_gemma":[0.000015310137,0.00024045461,0.074111395,0.000010164378,0.000021846909,0.0004883988,0.00018005146,0.0020159502,0.9173952,0.0004673174,0.0050346754,0.0000193387],"about_ca_topic_score_codex":0.0010830532,"about_ca_topic_score_gemma":0.0012757672,"teacher_disagreement_score":0.0010830532,"about_ca_system_score_codex":0.00023534597,"about_ca_system_score_gemma":0.000095951145,"threshold_uncertainty_score":0.0026683211},"labels":[],"label_agreement":null},{"id":"W2008017324","doi":"10.1088/0004-637x/726/1/4","title":"STRUCTURE IN THE ROTATION MEASURE SKY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Sky; Line-of-sight; Rotation (mathematics); Faraday effect; Measure (data warehouse); Asymmetry; Latitude; Line (geometry); Differential rotation","score_opus":0.005520453455275023,"score_gpt":0.21302884390811594,"score_spread":0.20750839045284092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008017324","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9218583,0.0015036397,0.021574555,0.00025189767,0.000037826052,0.00005486061,0.014343705,0.00053299096,0.039842267],"genre_scores_gemma":[0.98842174,0.00018623016,0.0033515242,0.000023170538,0.000023777357,0.000019607127,0.006912763,0.000055571094,0.001005555],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993237,0.00016387505,0.000041763935,0.00015822826,0.00018997387,0.0001223966],"domain_scores_gemma":[0.998787,0.00023700393,0.000341933,0.00026697814,0.0002653245,0.0001018119],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005847472,0.00025935573,0.00036392838,0.0035405888,0.00040690054,0.0014496958,0.00024535545,0.0001368012,0.0055583185],"category_scores_gemma":[0.0024548161,0.00011059019,0.00035848242,0.0040373146,0.00040013247,0.0005550351,0.00085671945,0.00034328675,0.0010495521],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002792376,0.000038198916,0.72271454,0.00013996549,0.00023072756,0.00019624327,0.0008080478,0.006374871,0.011659565,0.040822487,0.007032895,0.20970322],"study_design_scores_gemma":[0.000011906952,0.00008597503,0.96084577,0.0000200435,0.00003524658,0.00035166086,0.00023178528,0.0047530504,0.0011771667,0.006637486,0.025830837,0.000019001398],"about_ca_topic_score_codex":0.00504144,"about_ca_topic_score_gemma":0.0033570458,"teacher_disagreement_score":0.0055583185,"about_ca_system_score_codex":0.0005566324,"about_ca_system_score_gemma":0.00037583234,"threshold_uncertainty_score":0.018594384},"labels":[],"label_agreement":null},{"id":"W2008033660","doi":"10.1088/0004-637x/792/1/45","title":"OPTICAL SPECTROSCOPY AND VELOCITY DISPERSIONS OF GALAXY CLUSTERS FROM THE SPT-SZ SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"Science and Technology Facilities Council; Jet Propulsion Laboratory; Office of Science; McGill University; University of Chicago; Smithsonian Astrophysical Observatory; Massachusetts Institute of Technology; Australian Government; California Institute of Technology; U.S. Department of Energy; Gordon and Betty Moore Foundation; Kavli Institute for Cosmological Physics, University of Chicago; Canada Research Chairs; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Velocity dispersion; Physics; Astrophysics; Galaxy cluster; Galaxy; Scaling; Redshift; Cluster (spacecraft); Spectroscopy; Astronomy","score_opus":0.00844250853527944,"score_gpt":0.2162170457849023,"score_spread":0.20777453724962286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008033660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971083,0.000073088,0.00004271394,0.000042622585,0.000002927303,0.0000025725283,0.0019596773,0.000007949202,0.00076013093],"genre_scores_gemma":[0.9941995,0.00010503201,0.00008663072,0.000016749647,0.0000075696425,0.000004235306,0.0048326687,0.0000056165322,0.000741979],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988186,0.000014527541,0.000008559372,0.000030811316,0.000035685352,0.00002857211],"domain_scores_gemma":[0.99933535,0.000052338673,0.00021236236,0.000057351535,0.00014352023,0.00019895316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020844121,0.00013314233,0.00014269027,0.0020250394,0.00029723553,0.00046073433,0.00022371372,0.00018917804,0.0019570207],"category_scores_gemma":[0.00086729816,0.00012499961,0.00014118609,0.001960327,0.000185694,0.00027465308,0.0007525295,0.00018185661,0.0005311546],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004451851,0.000014528277,0.99416554,0.000007260491,0.000028174893,0.000021351048,0.00015123199,0.00013698105,0.00066572573,0.00009297489,0.00089389423,0.0037776532],"study_design_scores_gemma":[7.7609144e-7,0.000004097454,0.99942327,0.0000012736247,0.0000038286703,0.000018047069,0.00010496452,0.000060859387,0.00002559107,0.000013620017,0.0003429286,8.5789316e-7],"about_ca_topic_score_codex":0.045619845,"about_ca_topic_score_gemma":0.080093,"teacher_disagreement_score":0.045619845,"about_ca_system_score_codex":0.00030627317,"about_ca_system_score_gemma":0.0002942162,"threshold_uncertainty_score":0.09070861},"labels":[],"label_agreement":null},{"id":"W2008126830","doi":"10.1088/0004-637x/776/1/60","title":"DEEP MULTI-TELESCOPE PHOTOMETRY OF NGC 5466. I. BLUE STRAGGLERS AND BINARY SYSTEMS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Globular cluster; Blue straggler; Photometry (optics); Binary star; Stars; Binary number; Star cluster; Cluster (spacecraft)","score_opus":0.011844415608240549,"score_gpt":0.22426003254441235,"score_spread":0.2124156169361718,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008126830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953367,0.00015203579,0.0005277564,0.00002199678,0.0000047499743,0.0000067490346,0.00185956,0.00006905431,0.0020213504],"genre_scores_gemma":[0.9952899,0.00008504027,0.0012176689,0.000015463193,0.0000087583785,0.0000057698035,0.0022961749,0.00002225842,0.001058982],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998622,0.000009021821,0.000007853244,0.000046371824,0.000036302572,0.000038183254],"domain_scores_gemma":[0.9997017,0.0000147851515,0.00008871776,0.00005190797,0.000038307582,0.00010468981],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000182896,0.00035103763,0.00024430547,0.0019115409,0.00036147202,0.00036968585,0.0002255806,0.00022642531,0.0020663894],"category_scores_gemma":[0.0003259,0.00019034634,0.0002459229,0.0012531894,0.00014090163,0.00027668447,0.00059602107,0.00022560102,0.0007509359],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001659296,0.00006050274,0.8997886,0.00005518044,0.00005353232,0.00030361343,0.0006406793,0.0015815796,0.07219743,0.00029905376,0.0012267134,0.023627153],"study_design_scores_gemma":[0.0000012689089,0.000014441914,0.99842143,0.0000025539503,0.0000058310884,0.00009048709,0.000049452025,0.0002987212,0.0003938041,0.000029155166,0.000689566,0.0000033543167],"about_ca_topic_score_codex":0.014856327,"about_ca_topic_score_gemma":0.031947166,"teacher_disagreement_score":0.014856327,"about_ca_system_score_codex":0.00043482092,"about_ca_system_score_gemma":0.00018071715,"threshold_uncertainty_score":0.029539704},"labels":[],"label_agreement":null},{"id":"W2008182803","doi":"10.1086/589136","title":"Can Gravitational Infall Energy Lead to the Observed Velocity Dispersion in DLAs?","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Velocity dispersion; Astrophysics; Halo; Dispersion (optics); Galaxy; Star formation; Gravitation; Interstellar medium; Gravitational potential; Range (aeronautics); Gravitational collapse; Computational physics; Astronomy; Optics","score_opus":0.01535929107188681,"score_gpt":0.20893260410348025,"score_spread":0.19357331303159345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008182803","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99661,0.00014476477,0.0013980938,0.00027364655,0.000011394232,0.0000043291416,0.00007379891,0.000053236174,0.0014308065],"genre_scores_gemma":[0.99966764,0.000027450642,0.00017606124,0.000016779406,0.000002127257,0.0000010734136,0.000025056906,0.0000042013016,0.000079571706],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999291,0.000013887874,0.0000050045337,0.000018714056,0.000008490782,0.000024904633],"domain_scores_gemma":[0.9994555,0.00017603915,0.00016556094,0.000056613142,0.000032176395,0.00011402942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003091758,0.00031918046,0.00020265974,0.00047507745,0.00033551035,0.00089473673,0.00042612114,0.00048460258,0.00089179905],"category_scores_gemma":[0.0032981357,0.00022629992,0.00033324127,0.0002922556,0.00046382737,0.0007121948,0.00065412687,0.00041448243,0.0001992118],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032585714,0.00006356722,0.91268504,0.000060386486,0.00009930209,0.00048109444,0.00051670143,0.041874442,0.019838585,0.009283002,0.00046459003,0.014307434],"study_design_scores_gemma":[0.00008946108,0.0001637111,0.62107694,0.00003841752,0.00010761406,0.000421921,0.00059209694,0.34759003,0.0105678,0.017405558,0.001898879,0.000047600857],"about_ca_topic_score_codex":0.009246846,"about_ca_topic_score_gemma":0.0069000307,"teacher_disagreement_score":0.009246846,"about_ca_system_score_codex":0.00078118854,"about_ca_system_score_gemma":0.00018733101,"threshold_uncertainty_score":0.018386066},"labels":[],"label_agreement":null},{"id":"W2008218714","doi":"10.1086/430168","title":"Imaging of SDSS<i>z</i>&gt; 6 Quasar Fields: Gravitational Lensing, Companion Galaxies, and the Host Dark Matter Halos","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Dark matter; Halo; Gravitation; Dark matter halo; Scalar field dark matter; Gravitational lens; Dark galaxy","score_opus":0.0057275366969427284,"score_gpt":0.2071360037501862,"score_spread":0.20140846705324347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008218714","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9587156,0.001675736,0.0014233735,0.0019474272,0.00017273656,0.00005009271,0.007497583,0.00054595986,0.027971618],"genre_scores_gemma":[0.97120667,0.000920726,0.0030316736,0.00035895614,0.00044400516,0.000011091351,0.006149373,0.00012301131,0.017754652],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997968,0.000012955461,0.00001431141,0.00004247239,0.000085469605,0.000048007423],"domain_scores_gemma":[0.9985178,0.00010957162,0.00033676837,0.00010841483,0.00043002042,0.00049744756],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058728264,0.00020969508,0.00026759072,0.002274087,0.00044831578,0.00082069385,0.0003265385,0.00054151926,0.016976364],"category_scores_gemma":[0.0011827591,0.0002884161,0.00025086128,0.0010238761,0.0002054276,0.00070643553,0.0004561226,0.00024345212,0.0025950873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092748564,0.00023119609,0.6357845,0.0005404899,0.00017698226,0.0012096561,0.0006002526,0.00043066635,0.18093668,0.001359328,0.05142154,0.12638125],"study_design_scores_gemma":[0.00003827657,0.000063978376,0.97097427,0.0000310421,0.000041323223,0.0010230094,0.00015473504,0.0003891556,0.012115279,0.00040977506,0.01474352,0.000015539954],"about_ca_topic_score_codex":0.0023281479,"about_ca_topic_score_gemma":0.0076766303,"teacher_disagreement_score":0.016976364,"about_ca_system_score_codex":0.00024840602,"about_ca_system_score_gemma":0.0002411776,"threshold_uncertainty_score":0.056791544},"labels":[],"label_agreement":null},{"id":"W2008283300","doi":"10.1086/590656","title":"Probing the Magnetized Interstellar Medium Surrounding the Planetary Nebula Sh 2‐216","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Interstellar medium; Planetary nebula; Nebula; Dark nebula; Emission nebula; Protoplanetary nebula; Stars; Ultraviolet astronomy","score_opus":0.015692193804592903,"score_gpt":0.2202604309106593,"score_spread":0.2045682371060664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008283300","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9847424,0.0003191015,0.0003304366,0.0002814026,0.00009676167,0.000010734024,0.00024014291,0.000045936224,0.01393305],"genre_scores_gemma":[0.98670584,0.0001865809,0.00039596294,0.00014017844,0.000040598916,0.000006287138,0.00045784554,0.000018308512,0.012048419],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999578,0.000002269383,8.86395e-7,0.000013022896,0.0000140218635,0.000012034393],"domain_scores_gemma":[0.9999243,0.00000880454,0.000013301917,0.0000075141925,0.00001666958,0.000029289498],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000086035434,0.00010175881,0.00011666531,0.00021949311,0.00048715892,0.00048627722,0.00019601906,0.0004062771,0.008817983],"category_scores_gemma":[0.00024751827,0.00013350337,0.00006947956,0.00012848819,0.00014507733,0.00028188998,0.00038903474,0.0002351587,0.0014950446],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026468534,0.000041950607,0.031156356,0.000048856724,0.000014632898,0.00053160905,0.00011517484,0.00009393118,0.9575889,0.00041702503,0.0020004385,0.0077264765],"study_design_scores_gemma":[0.000115296876,0.00085571693,0.66214114,0.000022753198,0.00004998384,0.0013695547,0.0012035564,0.0016920146,0.2908186,0.0008242604,0.04088352,0.000023499026],"about_ca_topic_score_codex":0.0007678037,"about_ca_topic_score_gemma":0.0020554075,"teacher_disagreement_score":0.008817983,"about_ca_system_score_codex":0.00012762415,"about_ca_system_score_gemma":0.00012174871,"threshold_uncertainty_score":0.029499054},"labels":[],"label_agreement":null},{"id":"W2008296801","doi":"10.1088/0004-637x/784/1/82","title":"ALMA OBSERVATIONS OF THE ORION PROPLYDS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; National Research Council Canada","funders":"","keywords":"Physics; Orion Nebula; Submillimeter Array; Astrophysics; Stars; Millimeter; Planet; Astronomy; Nebula; Spitzer Space Telescope; Photoevaporation; Exoplanet; Circumstellar disk; Protoplanetary disk; Star formation","score_opus":0.01690758373589594,"score_gpt":0.23139557141558653,"score_spread":0.2144879876796906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008296801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962029,0.0001618865,0.00024067731,0.000029447021,0.00000681669,0.000011366498,0.00046227433,0.00007168027,0.0028130894],"genre_scores_gemma":[0.99638927,0.00010444448,0.0013169501,0.000035442605,0.000033210163,0.000011893862,0.0013171899,0.000011959513,0.0007794991],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986184,0.000008776796,0.0000041324115,0.00004969857,0.000044764496,0.000030690637],"domain_scores_gemma":[0.99977356,0.000023938836,0.000058654936,0.000029589397,0.000036839145,0.0000774398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015507876,0.0002197249,0.00015057142,0.0009699234,0.00050420855,0.0004139835,0.00043430994,0.00025405054,0.00096713053],"category_scores_gemma":[0.00031246597,0.00017326818,0.00016106869,0.00045518484,0.00018119389,0.00030693552,0.00052803074,0.0002665427,0.0002702304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006151117,0.00016398123,0.8087147,0.000121073834,0.00013456824,0.00094327884,0.0011800625,0.0010936508,0.13467796,0.00051548495,0.0031644506,0.04867573],"study_design_scores_gemma":[0.000023977722,0.00010040272,0.9911082,0.000011123317,0.000029139272,0.0003044849,0.00012345695,0.0011724824,0.0026010019,0.00010684369,0.004409758,0.000009119353],"about_ca_topic_score_codex":0.004218431,"about_ca_topic_score_gemma":0.007406725,"teacher_disagreement_score":0.004218431,"about_ca_system_score_codex":0.00041272433,"about_ca_system_score_gemma":0.00013834679,"threshold_uncertainty_score":0.008387744},"labels":[],"label_agreement":null},{"id":"W2008492178","doi":"10.1086/378498","title":"Erratum: “CO Molecular Gas in Infrared Luminous Galaxies” (ApJ, 588, 771 [2003])","year":2003,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy","score_opus":0.006771947464413094,"score_gpt":0.245146064136802,"score_spread":0.23837411667238892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008492178","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011767609,0.0049116667,0.0008448331,0.041725017,0.94266254,0.000049629027,0.0019007031,0.00043632934,0.006292575],"genre_scores_gemma":[0.02803475,0.025303943,0.0068504694,0.17669477,0.42282256,0.00033161233,0.010857204,0.0015798864,0.3275248],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9991678,0.000107314096,0.00023021862,0.00016600285,0.0002532323,0.00007544817],"domain_scores_gemma":[0.99273694,0.0010781972,0.00073799584,0.00052496296,0.0043953457,0.0005265042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014015904,0.0025088296,0.0012760995,0.003991262,0.002451755,0.0024115397,0.002414871,0.004236704,0.030183194],"category_scores_gemma":[0.01368819,0.0009762927,0.0010703421,0.0030434856,0.0012222222,0.0025928803,0.0014097658,0.0045953095,0.03330838],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045774792,0.0000167135,0.0006589201,0.00013505008,0.00001767393,0.00031058808,0.000026794813,0.000038131693,0.00012005727,0.00032279422,0.98911965,0.009187938],"study_design_scores_gemma":[0.000062983,0.00009467655,0.01085971,0.00043594989,0.00007889223,0.0012308047,0.00018755345,0.00035550713,0.00058490044,0.0010994335,0.98494256,0.0000669445],"about_ca_topic_score_codex":0.019735329,"about_ca_topic_score_gemma":0.020160446,"teacher_disagreement_score":0.030183194,"about_ca_system_score_codex":0.0015553213,"about_ca_system_score_gemma":0.0016947461,"threshold_uncertainty_score":0.10097283},"labels":[],"label_agreement":null},{"id":"W2008536161","doi":"10.1088/0004-637x/768/2/137","title":"NONLINEAR COLOR-METALLICITY RELATIONS OF GLOBULAR CLUSTERS. IV. TESTING THE NONLINEARITY SCENARIO FOR COLOR BIMODALITY VIA<i>HST</i>/WFC3<i>u</i>-BAND PHOTOMETRY OF M84 (NGC 4374)","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Bimodality; Photometry (optics); Globular cluster; Galaxy; Metallicity; Elliptical galaxy; Monte Carlo method","score_opus":0.014653019470823047,"score_gpt":0.23344713251514607,"score_spread":0.21879411304432303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008536161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99672556,0.00008287798,0.0012558192,0.00004837961,0.0000013632315,0.0000061552837,0.00023571223,0.000047317797,0.0015968409],"genre_scores_gemma":[0.9993325,0.000013445427,0.0003689006,0.000009302013,0.0000017182905,0.0000018211249,0.00016051246,0.000004788129,0.000107091095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998288,0.000025329724,0.000009731415,0.00006904138,0.000031660013,0.000035248566],"domain_scores_gemma":[0.9983367,0.00039467032,0.0005774615,0.00028769602,0.00022276802,0.00018069643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000441075,0.00021995738,0.000107736174,0.0012628764,0.0003065881,0.0005672408,0.00026835437,0.00028034352,0.00095394615],"category_scores_gemma":[0.0026363065,0.00015184685,0.00021441068,0.0006855724,0.00059164857,0.0007323236,0.00088619953,0.0003577861,0.00027652676],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010734244,0.0000105336,0.978378,0.000015814074,0.00003095395,0.000054268494,0.0002571907,0.0030601963,0.009526708,0.0017214114,0.00020894803,0.006628539],"study_design_scores_gemma":[0.000007886369,0.000030001946,0.9756807,0.0000065654845,0.000014722483,0.00008948499,0.00018085985,0.017816653,0.0026545723,0.0031194142,0.0003880047,0.000011064341],"about_ca_topic_score_codex":0.008661054,"about_ca_topic_score_gemma":0.008735002,"teacher_disagreement_score":0.008661054,"about_ca_system_score_codex":0.0006633827,"about_ca_system_score_gemma":0.00018986581,"threshold_uncertainty_score":0.017221272},"labels":[],"label_agreement":null},{"id":"W2008548976","doi":"10.1086/591542","title":"The Evolution of Dusty Star Formation and Stellar Mass Assembly in Clusters: Results from the IRAC 3.6, 4.5, 5.8, and 8.0 μm Cluster Luminosity Functions","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Redshift; Galaxy cluster; Galaxy; Cluster (spacecraft); Population; Astronomy; Stellar mass; Star formation; Star cluster","score_opus":0.009804124754471118,"score_gpt":0.19772671058983046,"score_spread":0.18792258583535934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008548976","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992052,0.000030617408,0.00007028944,0.000009937857,3.927913e-7,0.000001240438,0.0004570989,0.00001730869,0.00020796263],"genre_scores_gemma":[0.9986842,0.000011386837,0.00011907719,0.0000037270843,0.0000017124594,0.000002100117,0.0010198334,0.0000088152165,0.00014923024],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998242,0.000021883978,0.00000776335,0.00005735229,0.000041744024,0.000047118887],"domain_scores_gemma":[0.99877936,0.00031408612,0.00037974675,0.00013569464,0.00015462107,0.00023651375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047157402,0.00021675123,0.0002264048,0.0014193428,0.00032549354,0.0005633896,0.00032754088,0.00025700865,0.00091051357],"category_scores_gemma":[0.0015510928,0.00015920917,0.0003816292,0.0007783248,0.00021844546,0.00022138389,0.0004485969,0.0001958974,0.0003459113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008166968,0.000019510608,0.9931068,0.000005783656,0.000041111907,0.000029790015,0.00010308805,0.0025850367,0.0011869188,0.000079328594,0.00025015435,0.0025108194],"study_design_scores_gemma":[0.0000018168436,0.0000093310755,0.99737775,0.0000011162973,0.0000092697865,0.000016286835,0.00003788204,0.0022516444,0.00016492253,0.000027003402,0.00010027557,0.0000027823605],"about_ca_topic_score_codex":0.022779584,"about_ca_topic_score_gemma":0.017952476,"teacher_disagreement_score":0.022779584,"about_ca_system_score_codex":0.00049537775,"about_ca_system_score_gemma":0.00018600625,"threshold_uncertainty_score":0.045293987},"labels":[],"label_agreement":null},{"id":"W2008555661","doi":"10.1088/0004-637x/785/2/123","title":"HIGH-RESOLUTION THREE-DIMENSIONAL SIMULATIONS OF CORE-COLLAPSE SUPERNOVAE IN MULTIPLE PROGENITORS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Supernova; Instability; Neutrino; Accretion (finance); Convection; Shock (circulatory); Stars; Circular symmetry","score_opus":0.024784695181302514,"score_gpt":0.2739222936569682,"score_spread":0.24913759847566566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008555661","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98640895,0.0001805248,0.0057116677,0.00038777938,0.00004613414,0.000046001325,0.00072029483,0.00018949588,0.00630914],"genre_scores_gemma":[0.99060774,0.0001491791,0.007518647,0.00015196987,0.000021670568,0.000078303885,0.00073536445,0.00007428837,0.00066281814],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999814,0.000048966147,0.000014376031,0.000022582188,0.000054650747,0.0000453272],"domain_scores_gemma":[0.99864644,0.00072931126,0.00015301882,0.00009596599,0.00014730768,0.00022809372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005405353,0.0005151591,0.00076735415,0.00053036265,0.00079751766,0.0010913876,0.0013999236,0.0012506208,0.0016319761],"category_scores_gemma":[0.0027586534,0.00047925406,0.0010803882,0.0006548539,0.00093129475,0.0004966141,0.0010590334,0.0012727646,0.00016949202],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013487984,0.00014186792,0.008497173,0.000033788845,0.00006336098,0.00016790134,0.00012334061,0.985509,0.0012776123,0.002590026,0.00033691252,0.0011241288],"study_design_scores_gemma":[0.000049462018,0.000031872616,0.0024008658,0.0000072367675,0.00000929277,0.000019197365,0.00005789743,0.9959013,0.0002985187,0.0009807117,0.00023287826,0.000010794864],"about_ca_topic_score_codex":0.020135151,"about_ca_topic_score_gemma":0.014335925,"teacher_disagreement_score":0.020135151,"about_ca_system_score_codex":0.0011591524,"about_ca_system_score_gemma":0.0010693463,"threshold_uncertainty_score":0.040035903},"labels":[],"label_agreement":null},{"id":"W2008573855","doi":"10.1088/0004-637x/797/2/110","title":"THE EFFECT OF NONLINEAR LANDAU DAMPING ON ULTRARELATIVISTIC BEAM PLASMA INSTABILITIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Landau damping; Instability; Equipartition theorem; Beam (structure); Two-stream instability; Wavelength; Nonlinear system; Oblique case; Plasma; Computational physics; Quantum electrodynamics; Extragalactic background light; Wavenumber; Mechanics; Optics; Astrophysics; Quantum mechanics; Magnetic field; Redshift; Galaxy","score_opus":0.004468925289419593,"score_gpt":0.2097011129171613,"score_spread":0.2052321876277417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008573855","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9853888,0.00033545526,0.0074390722,0.00014769965,0.000019292742,0.000010054394,0.00002298059,0.00011650024,0.0065202583],"genre_scores_gemma":[0.9992661,0.000070262766,0.00039287313,0.00000627737,0.00000304409,0.0000025193058,0.0000054104307,0.000011599045,0.00024189582],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991286,0.000025695068,0.0000032106293,0.000010682693,0.000021437485,0.000026106603],"domain_scores_gemma":[0.9993297,0.00041335422,0.000106206455,0.00005093786,0.00003895468,0.000060822764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019927316,0.0003532247,0.00024097094,0.00031278367,0.00039657726,0.0005477011,0.0003460091,0.0002659545,0.0016627484],"category_scores_gemma":[0.0018253729,0.0001494245,0.0002288383,0.00012846784,0.0006057096,0.0004439157,0.00058241823,0.00032431708,0.00020571965],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075995096,0.00019074378,0.03494511,0.00036395327,0.00015185133,0.0018613723,0.000665706,0.61063963,0.26647538,0.060947075,0.00096297543,0.022036266],"study_design_scores_gemma":[0.000062299136,0.00012665609,0.007154995,0.000013404616,0.000031979453,0.00016538314,0.00008476116,0.94684803,0.039885506,0.0049920036,0.0006077261,0.00002722255],"about_ca_topic_score_codex":0.0011489048,"about_ca_topic_score_gemma":0.00053113996,"teacher_disagreement_score":0.0016627484,"about_ca_system_score_codex":0.0003698614,"about_ca_system_score_gemma":0.00018294569,"threshold_uncertainty_score":0.0055624843},"labels":[],"label_agreement":null},{"id":"W2008715267","doi":"10.1088/0004-637x/729/2/131","title":"<i>CHANDRA</i>AND<i>RXTE</i>OBSERVATIONS OF 1E 1547.0–5408: COMPARING THE 2008 AND 2009 OUTBURSTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Pulsar; Context (archaeology); Observatory; Astronomy; Flux (metallurgy)","score_opus":0.041822434237711176,"score_gpt":0.2910781844347531,"score_spread":0.2492557501970419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008715267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979196,0.000096377575,0.00007151035,0.00004815128,0.000008219984,0.000006223871,0.00077694596,0.00002528261,0.0010476643],"genre_scores_gemma":[0.9941188,0.00019831062,0.00079868286,0.00006854648,0.00004990321,0.000015213031,0.004406315,0.00003079618,0.00031343938],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998292,0.000018168861,0.000016690088,0.000047525376,0.000032287175,0.00005610169],"domain_scores_gemma":[0.9988281,0.00016888005,0.0005952832,0.00013089327,0.000120303564,0.00015666365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031576908,0.0002624792,0.00037444918,0.001864619,0.00047164175,0.000640411,0.00046105767,0.0004428413,0.00078090496],"category_scores_gemma":[0.0011305738,0.00018831258,0.00029265712,0.0009283048,0.00040746882,0.00048061737,0.00093561,0.0004671837,0.0003869029],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059565715,0.00028151346,0.95108587,0.00010104664,0.00017056572,0.00064073905,0.0005382807,0.00094210624,0.026037874,0.00031514786,0.0027093652,0.01658174],"study_design_scores_gemma":[0.000009865334,0.00004667902,0.99728954,0.000007708215,0.00003190934,0.0002683465,0.00009643409,0.00028612808,0.0011615222,0.000042661206,0.0007475705,0.000011801651],"about_ca_topic_score_codex":0.008582547,"about_ca_topic_score_gemma":0.02247471,"teacher_disagreement_score":0.008582547,"about_ca_system_score_codex":0.00042429345,"about_ca_system_score_gemma":0.00018666612,"threshold_uncertainty_score":0.017065167},"labels":[],"label_agreement":null},{"id":"W2008720744","doi":"10.1086/308143","title":"The Resolved Narrow‐Line Region in NGC 4151","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Space Telescope Imaging Spectrograph; Astrophysics; Velocity dispersion; Galaxy; Astronomy; Population; Line (geometry); Outflow; Spectral line; Radial velocity; Hubble space telescope; Stars; Geometry","score_opus":0.00879069720805915,"score_gpt":0.2121032878960505,"score_spread":0.20331259068799137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008720744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99746156,0.00013648147,0.00024791024,0.000017347418,0.0000038334706,0.0000020389955,0.00026950575,0.00005597845,0.0018053608],"genre_scores_gemma":[0.9985135,0.00003175974,0.0003390165,0.0000137748375,0.0000026150458,0.0000022165136,0.0006762187,0.000008447496,0.0004124837],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998765,0.0000073697674,0.000006358568,0.00005332073,0.00002867509,0.000027805867],"domain_scores_gemma":[0.9997632,0.000020417765,0.00008522386,0.00003734862,0.00003174428,0.00006211069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011105887,0.0001799645,0.00014789909,0.0006947344,0.0003737687,0.0006176853,0.00033393042,0.00022849622,0.0017136869],"category_scores_gemma":[0.0003041191,0.00017300388,0.00020204388,0.0005549153,0.0001506951,0.00023896943,0.0004118381,0.00021199125,0.0004070299],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037854275,0.00010594656,0.6579741,0.00011493802,0.00013336184,0.0012413496,0.0014881811,0.002313852,0.30056015,0.0009269457,0.0013759002,0.033386704],"study_design_scores_gemma":[0.000009422625,0.000041292093,0.98964894,0.000012002539,0.000032803462,0.00032577236,0.0002712715,0.001506882,0.005257639,0.000118251766,0.002764992,0.000010835285],"about_ca_topic_score_codex":0.008801549,"about_ca_topic_score_gemma":0.012231005,"teacher_disagreement_score":0.008801549,"about_ca_system_score_codex":0.00049482554,"about_ca_system_score_gemma":0.00017131929,"threshold_uncertainty_score":0.017500639},"labels":[],"label_agreement":null},{"id":"W2008742607","doi":"10.1086/320051","title":"The Relative Star Formation Histories of Spiral Bulges and Elliptical Galaxies in the Hubble Deep Fields","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Elliptical galaxy; Spiral galaxy; Redshift; Bulge; Astronomy; Galaxy; Star formation; Photometry (optics); Luminous infrared galaxy; Lenticular galaxy; Galaxy formation and evolution; Stars","score_opus":0.008326015979211544,"score_gpt":0.2099501064913269,"score_spread":0.20162409051211536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008742607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996018,0.00005784566,0.000038361475,0.000007804979,2.9342888e-7,6.606049e-7,0.00007588484,0.0000025416532,0.00021489873],"genre_scores_gemma":[0.99953616,0.000041517913,0.000047296668,0.0000035293456,0.0000010626964,9.0895236e-7,0.00016635016,0.000001119046,0.00020210967],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989545,0.000014071168,0.000004906627,0.000029411474,0.000013353122,0.000042852662],"domain_scores_gemma":[0.9990398,0.00024332188,0.00027019743,0.000098192584,0.00007989611,0.00026851593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042042029,0.00014566659,0.00013486693,0.0022654643,0.00036593035,0.0004907058,0.00016492417,0.00019581654,0.0012775443],"category_scores_gemma":[0.001543373,0.00020649786,0.00016213901,0.0006475161,0.00046460106,0.0005419589,0.00034181032,0.00019408746,0.00016994223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007695086,0.000014842169,0.99061537,0.000005854953,0.000017436738,0.000033475648,0.0004094089,0.00093922706,0.0025877685,0.00039282104,0.00006416671,0.00484274],"study_design_scores_gemma":[0.0000015809302,0.000011398514,0.99914885,0.0000019517136,0.000004356081,0.000021934593,0.000066645676,0.00044986716,0.00011017753,0.00011850008,0.0000623563,0.0000022001834],"about_ca_topic_score_codex":0.022652334,"about_ca_topic_score_gemma":0.031059505,"teacher_disagreement_score":0.022652334,"about_ca_system_score_codex":0.0009204245,"about_ca_system_score_gemma":0.00018011626,"threshold_uncertainty_score":0.045040965},"labels":[],"label_agreement":null},{"id":"W2008746044","doi":"10.1088/0004-637x/692/1/402","title":"MORPHOKINEMATIC PROPERTIES OF THE 21 μm SOURCE IRAS 07134+1005","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Torus; Submillimeter Array; Physics; Astrophysics; RADIUS; Bipolar outflow; Asymptotic giant branch; Radiative transfer; Outflow; Spectral energy distribution; Envelope (radar); Line (geometry); Jet (fluid); Interferometry; Circumstellar envelope; Astronomy; Geometry; Star formation; Stars; Optics; Galaxy","score_opus":0.011413431052282192,"score_gpt":0.21119334337755974,"score_spread":0.19977991232527756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008746044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877876,0.000026197136,0.00019209522,0.000012265302,0.0000015026794,0.0000033008653,0.00023136374,0.00004310598,0.0007112823],"genre_scores_gemma":[0.9982376,0.00002091324,0.0006799877,0.000009205297,0.0000036116455,0.000004715877,0.00085912406,0.000011350819,0.00017344292],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994195,0.0000063626117,0.0000017970186,0.000013931245,0.000019098787,0.000016875143],"domain_scores_gemma":[0.99988794,0.000012207908,0.00004688865,0.000011626071,0.000012485735,0.000028868943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012698356,0.00025505116,0.00019270279,0.00058959867,0.00028510066,0.0002681697,0.00032237842,0.00023974925,0.000757617],"category_scores_gemma":[0.00028458034,0.00012896629,0.00017249589,0.0003772754,0.00019331009,0.00017010499,0.00028376863,0.00021691354,0.00021202986],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050155865,0.000220627,0.62529534,0.00007645417,0.00009730978,0.0009701692,0.0004571964,0.007954011,0.33184305,0.0014631638,0.0016695289,0.029451648],"study_design_scores_gemma":[0.000016111071,0.00015887157,0.986522,0.0000048311595,0.000026617792,0.00041011593,0.000072672774,0.0058679427,0.0047704033,0.00018496685,0.001938692,0.000026698484],"about_ca_topic_score_codex":0.0042949035,"about_ca_topic_score_gemma":0.007136553,"teacher_disagreement_score":0.0042949035,"about_ca_system_score_codex":0.0005462257,"about_ca_system_score_gemma":0.00011855396,"threshold_uncertainty_score":0.008539796},"labels":[],"label_agreement":null},{"id":"W2008810925","doi":"10.1086/379339","title":"The Fate of Nonradiative Magnetized Accretion Flows: Magnetically Frustrated Convection","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs","keywords":"Physics; Accretion (finance); Polytrope; Magnetohydrodynamics; Convection; Buoyancy; Hydrostatic equilibrium; Astrophysics; RADIUS; Accretion disc; Mechanics; Magnetic field; Classical mechanics; Astronomy","score_opus":0.009779160956268608,"score_gpt":0.22471147504185546,"score_spread":0.21493231408558686,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008810925","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99169534,0.00011305205,0.0029324337,0.00047004438,0.00001953639,0.000011433324,0.000028152368,0.000053779797,0.0046762484],"genre_scores_gemma":[0.9994024,0.000025589587,0.00028510694,0.000024144765,0.000006123213,0.0000046098103,0.0000071634395,0.000004813784,0.00024000858],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992883,0.000021873871,0.0000019486806,0.000010326556,0.000007376391,0.000029688408],"domain_scores_gemma":[0.999681,0.00006324129,0.00006899076,0.00004673432,0.000019432422,0.00012065468],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028528774,0.00024454668,0.00030037513,0.00013641303,0.0009362164,0.0014596101,0.0006772226,0.0008335324,0.0012589721],"category_scores_gemma":[0.0014451507,0.00020182997,0.00018753027,0.00007207143,0.0012454357,0.0013476099,0.0009167726,0.00034378702,0.00017512997],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015574738,0.00039995403,0.034663282,0.00015651711,0.00011656082,0.0055392636,0.0018128733,0.3915865,0.04737699,0.5020377,0.0037708378,0.010982055],"study_design_scores_gemma":[0.00042791417,0.00019966313,0.0061565945,0.000018492634,0.000026239679,0.00046141158,0.00056382385,0.84162366,0.0035422507,0.14530995,0.0016185545,0.000051402],"about_ca_topic_score_codex":0.0012230251,"about_ca_topic_score_gemma":0.0005599193,"teacher_disagreement_score":0.0014596101,"about_ca_system_score_codex":0.00047960665,"about_ca_system_score_gemma":0.00032572792,"threshold_uncertainty_score":0.004211664},"labels":[],"label_agreement":null},{"id":"W2008975265","doi":"10.1088/0004-637x/754/2/132","title":"POLYCYCLIC AROMATIC HYDROCARBON PROCESSING IN THE BLAST WAVE OF THE SUPERNOVA REMNANT N132D","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Supernova; Blast wave; Supernova remnant; Interstellar medium; Shock wave; Plateau (mathematics); Polycyclic aromatic hydrocarbon; Astronomy; Molecular cloud; Infrared; Large Magellanic Cloud; Cosmic dust; Spectral line; Astrobiology; Galaxy; Stars","score_opus":0.015399667565846906,"score_gpt":0.23622675925851416,"score_spread":0.22082709169266726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008975265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99947876,0.00007182214,0.000035159323,0.000006740091,0.0000012449142,0.0000019749666,0.00008934839,0.000007263165,0.00030769903],"genre_scores_gemma":[0.9988949,0.00007026413,0.00020728413,0.00001218058,0.0000040295668,0.0000035296316,0.00047932405,0.000004002458,0.00032448434],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999962,0.0000018196133,0.0000019095664,0.000012352067,0.000012125927,0.000009837939],"domain_scores_gemma":[0.9999027,0.0000045014604,0.000032174892,0.000008779992,0.000008443636,0.000043379452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008840082,0.0002924599,0.00027883638,0.00043400386,0.00028923285,0.00024110172,0.00018335853,0.0001965901,0.0007213944],"category_scores_gemma":[0.000120538214,0.00015480764,0.00021586748,0.00031892495,0.00024051787,0.00013996828,0.00042128505,0.0002310414,0.0002468346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009560117,0.000104720886,0.5148459,0.00006914067,0.00008585826,0.0029090247,0.00045927416,0.000592036,0.47060698,0.00015225542,0.00031748146,0.008901335],"study_design_scores_gemma":[0.000008039819,0.00008387996,0.99596643,0.000002504907,0.000009909159,0.0004137181,0.00006623009,0.00023208155,0.002662344,0.000031619806,0.0005187754,0.000004514474],"about_ca_topic_score_codex":0.0060583055,"about_ca_topic_score_gemma":0.012370179,"teacher_disagreement_score":0.0060583055,"about_ca_system_score_codex":0.00035122424,"about_ca_system_score_gemma":0.00014817364,"threshold_uncertainty_score":0.012046099},"labels":[],"label_agreement":null},{"id":"W2008991538","doi":"10.1088/0004-637x/744/2/154","title":"GOODS-<i>HERSCHEL</i>MEASUREMENTS OF THE DUST ATTENUATION OF TYPICAL STAR-FORMING GALAXIES AT HIGH REDSHIFT: OBSERVATIONS OF ULTRAVIOLET-SELECTED GALAXIES AT<i>z</i>∼ 2","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":234,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"European Space Agency; Space Telescope Science Institute; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Luminous infrared galaxy; Galaxy; Redshift; Star formation; Astronomy; Submillimeter Array; Infrared; Ultraviolet","score_opus":0.031323177295176696,"score_gpt":0.21705592839031862,"score_spread":0.18573275109514192,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2008991538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99098164,0.0002125248,0.0011697586,0.000034525623,0.0000033212004,0.000008834872,0.0037552128,0.00023523027,0.0035989925],"genre_scores_gemma":[0.9931484,0.000097407734,0.0020861698,0.00004304798,0.00001320602,0.000009607264,0.003939312,0.000027460941,0.00063536386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998369,0.000011213472,0.000007737549,0.00005300257,0.000039113675,0.00005204601],"domain_scores_gemma":[0.9996177,0.000022371778,0.00017619082,0.00006850244,0.00003449818,0.00008061974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025197017,0.00030168498,0.00023831552,0.0013538722,0.00018632293,0.00061160227,0.00031394942,0.00022694771,0.0016861527],"category_scores_gemma":[0.00033554077,0.00026339848,0.0003126206,0.0008759104,0.00019554638,0.00036355367,0.00048507398,0.0002319324,0.00070269156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008713788,0.000043043015,0.9424262,0.000050206716,0.00009505334,0.000059655675,0.0001701855,0.0007374193,0.046476807,0.0003759924,0.0011972266,0.008281024],"study_design_scores_gemma":[0.0000027599588,0.00000913845,0.997341,0.0000013519034,0.000007738458,0.000034390476,0.000014123517,0.00021234518,0.0018321604,0.000041176263,0.0005015196,0.0000022742456],"about_ca_topic_score_codex":0.0050377958,"about_ca_topic_score_gemma":0.014060592,"teacher_disagreement_score":0.0050377958,"about_ca_system_score_codex":0.00048447974,"about_ca_system_score_gemma":0.00013290842,"threshold_uncertainty_score":0.010016918},"labels":[],"label_agreement":null},{"id":"W2009091432","doi":"10.1088/0004-637x/692/1/l19","title":"DO MODERATE-LUMINOSITY ACTIVE GALACTIC NUCLEI SUPPRESS STAR FORMATION?","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":168,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Supermassive black hole; Active galactic nucleus; Galaxy; Star formation; Black hole (networking); Intergalactic star; Intermediate-mass black hole; Stellar black hole","score_opus":0.014816832490831088,"score_gpt":0.24150066356103062,"score_spread":0.22668383107019952,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009091432","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9786199,0.003220142,0.002002568,0.0020711403,0.00017460063,0.00003224801,0.00023103003,0.00009333389,0.013555081],"genre_scores_gemma":[0.99722195,0.0006887527,0.0002616138,0.0004024664,0.000044793782,0.000007230384,0.00006266546,0.0000054212755,0.0013050307],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999095,0.000014091591,0.0000045702386,0.000025748139,0.000014145921,0.000031861033],"domain_scores_gemma":[0.9994475,0.000110137335,0.00022592982,0.000050769508,0.00004346652,0.00012221975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037267784,0.000115836476,0.00021968111,0.00008835405,0.00015198157,0.00053378363,0.00031545974,0.00042186296,0.0028775928],"category_scores_gemma":[0.0011833609,0.00010377304,0.0001271954,0.00007311575,0.0003808342,0.00048874685,0.00023497378,0.00021414936,0.0005868406],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003268269,0.0010757687,0.3858673,0.000964527,0.00043283883,0.001510167,0.0008196631,0.0016976551,0.400057,0.028758077,0.0064172945,0.16913141],"study_design_scores_gemma":[0.00035370747,0.0013395724,0.8739343,0.00010918105,0.00015654729,0.0011931516,0.001047569,0.002949919,0.0603867,0.016646368,0.041848566,0.000034421126],"about_ca_topic_score_codex":0.001538961,"about_ca_topic_score_gemma":0.0021946975,"teacher_disagreement_score":0.0028775928,"about_ca_system_score_codex":0.0002794943,"about_ca_system_score_gemma":0.00034508537,"threshold_uncertainty_score":0.009626508},"labels":[],"label_agreement":null},{"id":"W2009091478","doi":"10.1088/0004-637x/709/2/1067","title":"THE CFHTLS-DEEP CATALOG OF INTERACTING GALAXIES. I. MERGER RATE EVOLUTION TO<i>z</i>= 1.2","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Galaxy; Galaxy merger; Star formation; Galaxy formation and evolution; Stellar mass; Telescope; Fraction (chemistry); Mass ratio","score_opus":0.005023362158186754,"score_gpt":0.21613421828926296,"score_spread":0.21111085613107622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009091478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.59009767,0.0010917082,0.001400107,0.00023892638,0.00003331677,0.00012193882,0.38727733,0.0015030012,0.018236052],"genre_scores_gemma":[0.50172436,0.00038112298,0.0050360463,0.00020712486,0.00006141488,0.0001245145,0.48532122,0.00012402964,0.0070201335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978,0.000010406623,0.000010601639,0.000058042933,0.000068734305,0.00007219888],"domain_scores_gemma":[0.9989153,0.00006821149,0.00025006972,0.00015894958,0.00027463475,0.0003328285],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032134308,0.00037640458,0.00024304808,0.0052860905,0.00038280227,0.0004972339,0.0004544281,0.0002539827,0.0047602663],"category_scores_gemma":[0.0010236894,0.00017452321,0.0002980022,0.0028800908,0.00016063555,0.0005268636,0.00083569804,0.00026049098,0.001935131],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014531276,0.00005584032,0.8700341,0.00016209172,0.00011805105,0.00013424989,0.00043294777,0.0011234948,0.0072934497,0.0019671235,0.07510889,0.04342441],"study_design_scores_gemma":[0.000014825784,0.000019310373,0.95980674,0.000017084612,0.000023089638,0.00014059043,0.000087063374,0.0009032728,0.0006768676,0.00015667656,0.038143978,0.000010567082],"about_ca_topic_score_codex":0.09386073,"about_ca_topic_score_gemma":0.12368328,"teacher_disagreement_score":0.09386073,"about_ca_system_score_codex":0.0010531313,"about_ca_system_score_gemma":0.00091107853,"threshold_uncertainty_score":0.18662882},"labels":[],"label_agreement":null},{"id":"W2009096052","doi":"10.1086/323792","title":"The Masses of White Dwarfs in the Praesepe Open Cluster","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Pleiades; White dwarf; Astrophysics; Open cluster; Balmer series; Brown dwarf; Astronomy; Cluster (spacecraft); Spectral line; Massive compact halo object; Stars; Emission spectrum","score_opus":0.013762086601514198,"score_gpt":0.25606550241163983,"score_spread":0.24230341581012563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009096052","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965155,0.000025771267,0.00007517243,0.000003317797,2.7129383e-7,0.0000011887557,0.000040877785,0.0000035098474,0.00019827991],"genre_scores_gemma":[0.9988524,0.000047417318,0.00039167498,0.000003843461,0.0000016499995,0.0000033587262,0.00031333565,0.0000039921024,0.00038233324],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990356,0.000008060462,0.00000383726,0.000035361372,0.000023456934,0.000025688802],"domain_scores_gemma":[0.9997453,0.000049945582,0.00006790455,0.000027617183,0.00004017353,0.00006905906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017195003,0.00020326488,0.00016514825,0.00097027776,0.0006060543,0.00039069957,0.00027369897,0.00013593843,0.00036230052],"category_scores_gemma":[0.0006922273,0.00014238078,0.00010577779,0.00053939014,0.00047465746,0.0003931275,0.0007150706,0.00017796764,0.00019273644],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036777623,0.00008535104,0.94029367,0.000034171968,0.000060631217,0.00048612946,0.0030010438,0.00079811073,0.030074159,0.0007034213,0.00032395188,0.023771673],"study_design_scores_gemma":[0.0000063656294,0.00008670075,0.9951513,0.0000020245802,0.000011581032,0.00035204287,0.00042629393,0.00054845156,0.0020166845,0.00022377002,0.0011657658,0.000009058961],"about_ca_topic_score_codex":0.010442095,"about_ca_topic_score_gemma":0.01602647,"teacher_disagreement_score":0.010442095,"about_ca_system_score_codex":0.0003866638,"about_ca_system_score_gemma":0.00015699628,"threshold_uncertainty_score":0.020762682},"labels":[],"label_agreement":null},{"id":"W2009187400","doi":"10.1086/521351","title":"The Circumnuclear Molecular Gas in the Seyfert Galaxy NGC 4945","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; RADIUS; Galaxy rotation curve; Submillimeter Array; Dust lane; Star formation; Asymmetry; Active galactic nucleus; Astronomy; Galactic Center; Molecular cloud; Luminous infrared galaxy; Galaxy formation and evolution; Stars","score_opus":0.007117679758931633,"score_gpt":0.23669464675655366,"score_spread":0.22957696699762203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009187400","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99957484,0.0000470642,0.00007274128,0.0000058346586,6.971111e-7,0.0000010266893,0.00003438418,0.000006631198,0.00025680027],"genre_scores_gemma":[0.999724,0.000031994623,0.000106914835,0.0000042377437,0.0000016107732,7.6686644e-7,0.000060347575,9.913508e-7,0.00006914338],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993134,0.000008922706,0.0000031676411,0.00002472578,0.000013826415,0.000017982846],"domain_scores_gemma":[0.9998809,0.000013533823,0.00004266332,0.00001591209,0.000012720012,0.000034183104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000087017965,0.00013308838,0.00011117521,0.00054191344,0.00022026335,0.00037069691,0.0001380266,0.00012268535,0.00072409946],"category_scores_gemma":[0.00024520297,0.00008314256,0.00007552779,0.00036235838,0.00019072404,0.00023980984,0.0002761571,0.000068413734,0.000114735616],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015179286,0.00004958683,0.86079854,0.000021741176,0.00006349538,0.0005701787,0.0011236615,0.0014455881,0.11952642,0.0007780449,0.00022297958,0.015247949],"study_design_scores_gemma":[0.0000059777826,0.00004832319,0.9955869,0.0000043533773,0.000015141404,0.00019416925,0.00012816716,0.00091206643,0.0021388386,0.00011962591,0.0008428606,0.0000036161257],"about_ca_topic_score_codex":0.008264091,"about_ca_topic_score_gemma":0.0099956235,"teacher_disagreement_score":0.008264091,"about_ca_system_score_codex":0.00018003487,"about_ca_system_score_gemma":0.000065687826,"threshold_uncertainty_score":0.016431987},"labels":[],"label_agreement":null},{"id":"W2009270572","doi":"10.1086/340654","title":"Subarcsecond Mid‐Infrared Imaging of Two Post–Asymptotic Giant Branch 21 Micron Sources","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canada Council for the Arts; University of Calgary","funders":"","keywords":"Physics; Asymptotic giant branch; Astrophysics; Planetary nebula; Infrared; Feature (linguistics); Astronomy; Stars","score_opus":0.007624689559200499,"score_gpt":0.21680177683295965,"score_spread":0.20917708727375914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009270572","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976902,0.00008033708,0.00019041945,0.000028128123,0.000002431297,0.000004116235,0.00012129959,0.0000185109,0.0018646583],"genre_scores_gemma":[0.99681723,0.00007687628,0.0011924469,0.000029682291,0.000007400213,0.000007865069,0.0007746043,0.000009006448,0.001084739],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996734,0.0000014026297,0.0000011598328,0.00000691168,0.000010371308,0.0000127705225],"domain_scores_gemma":[0.9998779,0.000010991708,0.000029809768,0.000010268796,0.000020694557,0.00005024149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007104087,0.0001173355,0.00013165161,0.0006143876,0.00034502894,0.00019540175,0.00017580156,0.00031976128,0.0013453093],"category_scores_gemma":[0.00013942865,0.000117156174,0.0001197748,0.00021108965,0.000076324075,0.00011257312,0.0002735307,0.0002948694,0.00028899798],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048525404,0.00014770485,0.07199386,0.0000512747,0.000031616488,0.0015729954,0.00062720076,0.00031397463,0.90520644,0.00045777755,0.0006823722,0.018429438],"study_design_scores_gemma":[0.0000071384206,0.000045040935,0.9923207,0.000004000398,0.000008490807,0.0008322412,0.00005968656,0.00027139802,0.005371196,0.00004563601,0.0010300927,0.0000042568668],"about_ca_topic_score_codex":0.0022682757,"about_ca_topic_score_gemma":0.00701069,"teacher_disagreement_score":0.0022682757,"about_ca_system_score_codex":0.00033714593,"about_ca_system_score_gemma":0.00008588567,"threshold_uncertainty_score":0.0045101047},"labels":[],"label_agreement":null},{"id":"W2009367128","doi":"10.1088/0004-637x/799/2/181","title":"CAN THE MASSES OF ISOLATED PLANETARY-MASS GRAVITATIONAL LENSES BE MEASURED BY TERRESTRIAL PARALLAX?","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Gravitational microlensing; Gravitational lens; Mass distribution; Lens (geology); Event (particle physics); Stars; Parallax; Population; Orbit (dynamics)","score_opus":0.027812917093457633,"score_gpt":0.23936355531159859,"score_spread":0.21155063821814096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009367128","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9662013,0.006616998,0.014993322,0.0004867338,0.00008183316,0.000027128433,0.0008530441,0.00027996136,0.0104597565],"genre_scores_gemma":[0.9947984,0.0006869825,0.003363362,0.00011295742,0.0000778677,0.000012017622,0.00052302814,0.00003107932,0.00039413455],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9994659,0.000096553886,0.000028760598,0.00019272279,0.00013598164,0.000080166225],"domain_scores_gemma":[0.9936871,0.0015873364,0.003172165,0.00068550534,0.00039859227,0.00046925803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013231995,0.0008243647,0.00064122904,0.002615869,0.00056195015,0.0012420417,0.000992704,0.00073056284,0.0014605146],"category_scores_gemma":[0.006747648,0.00045174127,0.00044938395,0.0018820623,0.001138089,0.0025878192,0.001451478,0.0007447291,0.0009756567],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000329252,0.000029591478,0.9393175,0.00026305122,0.00050590164,0.00042744033,0.00070038426,0.00062730385,0.017996343,0.0014184014,0.0005763839,0.037808437],"study_design_scores_gemma":[0.000007687382,0.0001106554,0.9880144,0.000028433758,0.00007829757,0.0005217163,0.00034690383,0.0015544335,0.003453921,0.002465295,0.003389362,0.000028891936],"about_ca_topic_score_codex":0.0022205145,"about_ca_topic_score_gemma":0.0043846425,"teacher_disagreement_score":0.002615869,"about_ca_system_score_codex":0.00037950987,"about_ca_system_score_gemma":0.000097205,"threshold_uncertainty_score":0.0069978237},"labels":[],"label_agreement":null},{"id":"W2009404384","doi":"10.1086/506521","title":"Magnetic Field Decay and Period Evolution of Anomalous X-Ray Pulsarsin the Context of Quark Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Neutron star; Magnetic field; RADIUS; Context (archaeology); Stars; Pulsar; Field (mathematics); Period (music)","score_opus":0.005195079323872024,"score_gpt":0.2569410088598717,"score_spread":0.25174592953599967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009404384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971884,0.00006730776,0.0019596843,0.000036151978,0.0000025929776,0.0000017315787,0.000021509182,0.00001543382,0.00070721714],"genre_scores_gemma":[0.9993144,0.000050490824,0.00040224692,0.0000047797207,0.0000039476663,0.0000023658629,0.0000306636,0.0000060271814,0.00018507778],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99997354,0.0000060676643,0.0000015829504,0.0000059852837,0.000004508056,0.000008331558],"domain_scores_gemma":[0.9997234,0.00007399924,0.00011902876,0.000027213975,0.0000244988,0.000031728094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001509862,0.00023986747,0.00020355522,0.0003256658,0.00028040097,0.0004731964,0.00028962054,0.000254233,0.0006021747],"category_scores_gemma":[0.00095082057,0.00011771518,0.00019949503,0.00022897318,0.00047462372,0.00051998935,0.00034989978,0.00025151967,0.000082613355],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043468515,0.00011660422,0.23434088,0.00006713627,0.00010878955,0.0010532209,0.00042685342,0.6482025,0.054113504,0.051465087,0.00058552774,0.009085214],"study_design_scores_gemma":[0.000026130581,0.000064882115,0.031116055,0.0000053477083,0.00002508574,0.00015424285,0.0000887143,0.9593385,0.0035612194,0.005134155,0.00047079677,0.000014923128],"about_ca_topic_score_codex":0.0028039785,"about_ca_topic_score_gemma":0.001758315,"teacher_disagreement_score":0.0028039785,"about_ca_system_score_codex":0.0004813583,"about_ca_system_score_gemma":0.00019008589,"threshold_uncertainty_score":0.0055752993},"labels":[],"label_agreement":null},{"id":"W2009408083","doi":"10.1086/345929","title":"Correlations of Richness and Global Properties in Galaxy Clusters","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Redshift; Velocity dispersion; Galaxy cluster; Species richness; Galaxy; Cluster (spacecraft); RADIUS; Cosmology; Luminosity; Scaling; Astronomy; Geology","score_opus":0.008668977023142671,"score_gpt":0.20484998845405838,"score_spread":0.1961810114309157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009408083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973375,0.00013189937,0.0009206036,0.000025408572,0.0000018371869,0.0000044926837,0.00035446323,0.000036200167,0.0011875891],"genre_scores_gemma":[0.9994624,0.00002338937,0.00015880156,0.000004118139,0.0000036649953,0.0000019981646,0.0002482115,0.000005418041,0.00009200736],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955255,0.000089707195,0.00002136002,0.00014557707,0.00010838569,0.00008232622],"domain_scores_gemma":[0.9918869,0.003535983,0.0023771639,0.0008865243,0.0006228133,0.00069067476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007444967,0.00025106707,0.0003416126,0.0020420437,0.0002741513,0.00067837175,0.00022391218,0.00020816912,0.0013050205],"category_scores_gemma":[0.006959408,0.0002231877,0.0002081715,0.0012439769,0.0007817627,0.0006398714,0.0010656716,0.00037704833,0.00023931851],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055724184,0.000008000271,0.9914718,0.00000966955,0.000098236,0.000041862768,0.00012231602,0.003736649,0.0014944101,0.00039365873,0.00012461009,0.0024430915],"study_design_scores_gemma":[0.0000020150076,0.00001342823,0.99481577,0.0000041167236,0.000011935276,0.000052221407,0.00007416978,0.0041918224,0.00027714606,0.00042135277,0.00012775512,0.00000824365],"about_ca_topic_score_codex":0.0046895705,"about_ca_topic_score_gemma":0.0037584584,"teacher_disagreement_score":0.0046895705,"about_ca_system_score_codex":0.00030914132,"about_ca_system_score_gemma":0.00013493949,"threshold_uncertainty_score":0.009324551},"labels":[],"label_agreement":null},{"id":"W2009458597","doi":"10.1088/0004-637x/757/1/68","title":"<i>CHANDRA</i>OBSERVATIONS OF SGR 1627–41 NEAR QUIESCENCE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Flux (metallurgy); Pulsar; Observatory; Magnetic field; Photon; Power law; Luminosity; Astronomy; Galaxy","score_opus":0.025170444175031444,"score_gpt":0.31648306768537354,"score_spread":0.2913126235103421,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009458597","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99289495,0.0004263561,0.00035346733,0.00009872597,0.000024419758,0.000021083855,0.0015683239,0.00014613535,0.004466566],"genre_scores_gemma":[0.99148226,0.00034211105,0.0016389578,0.00013575223,0.00008249533,0.000016694123,0.005178451,0.000044294695,0.00107904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989367,0.000006583148,0.0000072991775,0.000023530012,0.00003684181,0.000032128515],"domain_scores_gemma":[0.99958724,0.000033873996,0.00014728036,0.00005652953,0.00005048183,0.00012454212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023262804,0.00034313902,0.00036688376,0.0011119371,0.0007938577,0.00048947765,0.00045290455,0.00043742926,0.0010903801],"category_scores_gemma":[0.0003492326,0.00018410431,0.00029683337,0.0007028292,0.00026159355,0.00037642,0.0005608591,0.00041703423,0.00050227373],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010956094,0.00042162233,0.72368324,0.0004984445,0.00032965755,0.009656486,0.0013991331,0.0023597295,0.21252261,0.0010759749,0.009294106,0.037663445],"study_design_scores_gemma":[0.000022297125,0.00024030381,0.98373544,0.00003093908,0.00003743129,0.0017153565,0.00015502622,0.00070046965,0.005770421,0.00017489777,0.0073877033,0.000029825014],"about_ca_topic_score_codex":0.004187049,"about_ca_topic_score_gemma":0.015171022,"teacher_disagreement_score":0.004187049,"about_ca_system_score_codex":0.00029639027,"about_ca_system_score_gemma":0.00023685714,"threshold_uncertainty_score":0.008325338},"labels":[],"label_agreement":null},{"id":"W2009482806","doi":"10.1088/0004-637x/747/1/5","title":"STATISTICAL DESCRIPTION OF SYNCHROTRON INTENSITY FLUCTUATIONS: STUDIES OF ASTROPHYSICAL MAGNETIC TURBULENCE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Synchrotron; Turbulence; Magnetic field; Anisotropy; Electron; Quadrupole; Turbulence kinetic energy; Synchrotron radiation","score_opus":0.02303724605130922,"score_gpt":0.26090101230120477,"score_spread":0.23786376624989555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009482806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6156021,0.0012380418,0.37467027,0.0008645558,0.000054271582,0.000038215607,0.000345539,0.000247057,0.0069399457],"genre_scores_gemma":[0.9943,0.00031923607,0.004492896,0.00003827369,0.000104280654,0.00002173693,0.00011481642,0.0000381047,0.00057055324],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999632,0.00011549798,0.000022734877,0.00005219294,0.00011038608,0.000067165245],"domain_scores_gemma":[0.9968618,0.0014107904,0.00081105094,0.00033347352,0.00041552758,0.00016731316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012758139,0.00035251823,0.00043097965,0.0012243108,0.0003803491,0.000848489,0.0007145232,0.00045141325,0.00060976506],"category_scores_gemma":[0.0056569837,0.00022645616,0.0003816281,0.001124248,0.0010591798,0.0012329369,0.00043695248,0.000463578,0.00010692406],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000093858725,0.00009093179,0.03728063,0.00011589056,0.000106074076,0.00048794,0.00027770252,0.48060122,0.01982373,0.44752526,0.0012170664,0.012379775],"study_design_scores_gemma":[0.00000723255,0.000030084999,0.013819706,0.000010199384,0.000008828523,0.00014651657,0.000038125203,0.9215419,0.0010904309,0.062716864,0.00056467426,0.000025466516],"about_ca_topic_score_codex":0.0017600298,"about_ca_topic_score_gemma":0.00085551053,"teacher_disagreement_score":0.0017600298,"about_ca_system_score_codex":0.0006919951,"about_ca_system_score_gemma":0.000530276,"threshold_uncertainty_score":0.006747186},"labels":[],"label_agreement":null},{"id":"W2009490864","doi":"10.1086/432032","title":"Unusual Pulsed X‐Ray Emission from the Young, High Magnetic Field Pulsar PSR J1119−6127","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Neutron star; Black-body radiation; RADIUS; Millisecond pulsar; Magnetic field; Dipole; Magnetic dipole; X-ray pulsar","score_opus":0.007963764157066318,"score_gpt":0.28649545195487225,"score_spread":0.2785316877978059,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009490864","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981914,0.00018960884,0.00026766025,0.000038569637,0.0000087348335,0.000004943066,0.00021968261,0.0000316236,0.0010477798],"genre_scores_gemma":[0.9976603,0.00023033607,0.00048778142,0.000043951182,0.000027865308,0.000012046266,0.0009605816,0.000024355253,0.00055285904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999217,0.0000054392917,0.0000051742113,0.000025472124,0.000024491374,0.000017869637],"domain_scores_gemma":[0.99978894,0.000029947214,0.00008184088,0.000023860024,0.000025844074,0.000049572394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012273683,0.00026709546,0.00029754202,0.00055358536,0.00035487794,0.0006229319,0.00040061222,0.00025896114,0.0009649796],"category_scores_gemma":[0.00030948577,0.00018629574,0.00013229807,0.00053228886,0.0003461973,0.00019416463,0.00047552874,0.00039174253,0.000501994],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005264852,0.00024203726,0.5505949,0.00026968162,0.00017638165,0.0054101287,0.00067410286,0.0011043141,0.40508193,0.00096098037,0.0037676385,0.031191448],"study_design_scores_gemma":[0.00006908737,0.0002563504,0.9681382,0.000024615496,0.000087424036,0.0058302344,0.0002917221,0.0016985852,0.014993214,0.00036784715,0.0082045905,0.000037962505],"about_ca_topic_score_codex":0.0010184287,"about_ca_topic_score_gemma":0.0019142311,"teacher_disagreement_score":0.0010184287,"about_ca_system_score_codex":0.0002382728,"about_ca_system_score_gemma":0.00014035747,"threshold_uncertainty_score":0.003228128},"labels":[],"label_agreement":null},{"id":"W2009567740","doi":"10.1086/423799","title":"The Location of the Core in M81","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Astrophysics; Physics; Very-long-baseline interferometry; Brightness; Core (optical fiber); Jet (fluid); Galaxy; Supernova; Spiral galaxy; Proper motion; Astronomy; Optics","score_opus":0.010106275627026465,"score_gpt":0.2246475181514196,"score_spread":0.21454124252439313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009567740","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973922,0.00017291105,0.00058655295,0.00001593631,0.0000023996959,0.0000031339928,0.00008701191,0.000024205488,0.0017156759],"genre_scores_gemma":[0.9990145,0.00004891337,0.00052456296,0.000012287306,0.0000048961974,0.000002598955,0.00018419354,0.0000049589275,0.00020316144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999145,0.000005491091,0.000003466125,0.000028132476,0.000017832805,0.00003046334],"domain_scores_gemma":[0.99978393,0.000023395844,0.0000900812,0.000027887472,0.000042077994,0.000032601176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014735531,0.00012805226,0.00016004205,0.0007262989,0.0003801472,0.00046211435,0.00025494394,0.0002639264,0.00068235426],"category_scores_gemma":[0.00038303333,0.00015050008,0.00009983317,0.0004742194,0.00017967558,0.00035915477,0.00059219636,0.0001837965,0.0003922431],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002753088,0.00007160282,0.84755373,0.000059651156,0.00003091387,0.0004431395,0.00120338,0.00065286394,0.10516164,0.0009275541,0.00082302897,0.042797256],"study_design_scores_gemma":[0.0000067619703,0.00006382077,0.99047333,0.000010410043,0.00001537938,0.00036622267,0.000119405515,0.0007954157,0.0058332267,0.00017910435,0.0021306574,0.000006302904],"about_ca_topic_score_codex":0.0021218958,"about_ca_topic_score_gemma":0.003934626,"teacher_disagreement_score":0.0021218958,"about_ca_system_score_codex":0.0002693294,"about_ca_system_score_gemma":0.0001185022,"threshold_uncertainty_score":0.0042191744},"labels":[],"label_agreement":null},{"id":"W2009568911","doi":"10.1088/0004-637x/784/1/7","title":"TESTING THE NO-HAIR THEOREM WITH EVENT HORIZON TELESCOPE OBSERVATIONS OF SAGITTARIUS A*","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":226,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Supermassive black hole; Kerr metric; Event horizon; Black hole (networking); Astrophysics; Spin-flip; Rotating black hole; Sagittarius A*; Binary black hole; Intermediate-mass black hole; Galactic Center; Astronomy; Accretion (finance); Schwarzschild radius; Gravitational wave; Galaxy; Event (particle physics)","score_opus":0.018366139056128897,"score_gpt":0.22144004514186472,"score_spread":0.20307390608573583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009568911","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99761033,0.00003089114,0.0011810246,0.00006132023,0.0000063876855,0.000010478855,0.000087682674,0.000043025913,0.0009688835],"genre_scores_gemma":[0.9985032,0.000014011311,0.0012233361,0.000018860484,0.000004857938,0.000004533886,0.00017796083,0.000013363529,0.00003981213],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995752,0.00014914731,0.00002233431,0.00008950644,0.000085418236,0.00007836997],"domain_scores_gemma":[0.9982346,0.00064932107,0.00036869163,0.00030258586,0.0001625701,0.00028220867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014664674,0.00033855118,0.0002734483,0.00031754817,0.00044568826,0.00071473303,0.0007817373,0.00048323377,0.0005860374],"category_scores_gemma":[0.004155417,0.00026581786,0.0005244666,0.000250503,0.00083423214,0.0005597555,0.00080675224,0.00041119396,0.000117926385],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018559388,0.0005404032,0.5118722,0.0001495716,0.0007694923,0.0012931136,0.00088940957,0.38608834,0.058012404,0.01633695,0.0015834768,0.020608712],"study_design_scores_gemma":[0.00024365119,0.000553481,0.21062332,0.000025281586,0.00009298505,0.00019980404,0.00029911814,0.7744944,0.007063737,0.004971932,0.0013652409,0.000067051056],"about_ca_topic_score_codex":0.01092361,"about_ca_topic_score_gemma":0.0069414317,"teacher_disagreement_score":0.01092361,"about_ca_system_score_codex":0.0008312125,"about_ca_system_score_gemma":0.00047357797,"threshold_uncertainty_score":0.021720111},"labels":[],"label_agreement":null},{"id":"W2009632868","doi":"10.1086/529131","title":"Simultaneous Multiwavelength Observations of Magnetic Activity in Ultracool Dwarfs. II. Mixed Trends in VB 10 and LSR 1835+32 and the Possible Role of Rotation","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Astrophysics; Physics; Luminosity; Stars; Rotation (mathematics); Rotation period; Starspot; Spectral line; Uncorrelated; Astronomy; Galaxy","score_opus":0.011833763793953051,"score_gpt":0.2178369043560164,"score_spread":0.20600314056206337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009632868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991653,0.00011219119,0.000085825195,0.000009111485,0.0000018981972,0.0000017759714,0.00019106909,0.000018157561,0.00041460615],"genre_scores_gemma":[0.9985341,0.000048173253,0.00046071495,0.000019905647,0.000006921495,0.000006115793,0.0006217058,0.0000068090226,0.0002956034],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999176,0.000006459207,0.0000042463166,0.000025561449,0.000019833411,0.000026254362],"domain_scores_gemma":[0.9997675,0.000020717309,0.0000920753,0.00001756668,0.000024942534,0.000077186356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011617506,0.00019587594,0.0001998602,0.00065867015,0.00025895349,0.00029191058,0.00024272273,0.00018464806,0.00061835354],"category_scores_gemma":[0.0002291527,0.0001709585,0.00015405664,0.00036853872,0.00016027142,0.00015804979,0.00037403035,0.00024059172,0.00022199367],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060359086,0.00007588619,0.7231824,0.00007518149,0.00010011992,0.0003624624,0.00074025925,0.00048795,0.2430079,0.0001525219,0.0004404899,0.030771298],"study_design_scores_gemma":[0.00001019769,0.00008931913,0.9968796,0.0000059657464,0.0000147558485,0.00018056302,0.00010257125,0.00023162804,0.0017645119,0.000031079362,0.0006857226,0.0000042073216],"about_ca_topic_score_codex":0.004418349,"about_ca_topic_score_gemma":0.017590376,"teacher_disagreement_score":0.004418349,"about_ca_system_score_codex":0.00036698504,"about_ca_system_score_gemma":0.00009358558,"threshold_uncertainty_score":0.008785248},"labels":[],"label_agreement":null},{"id":"W2009693179","doi":"10.1086/517882","title":"Can Astrophysical Gamma-Ray Sources Mimic Dark Matter Annihilation in Galactic Satellites?","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; WIMP; Dark matter; Weakly interacting massive particles; Astrophysics; Astronomy; Galactic halo; Cosmic ray; Baryonic dark matter; Light dark matter; Annihilation; Scalar field dark matter; Dark matter halo; Halo; Particle physics; Galaxy; Cosmology; Dark energy","score_opus":0.006821530227964999,"score_gpt":0.223253275134453,"score_spread":0.216431744906488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009693179","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98941106,0.00035934718,0.00522203,0.00023306557,0.00001631956,0.000012377234,0.00007423926,0.00010793398,0.0045636357],"genre_scores_gemma":[0.9982961,0.0001042011,0.0013069124,0.000037671212,0.000006527218,0.0000026595717,0.00003990821,0.000011091001,0.00019489175],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999032,0.000026918082,0.000005677345,0.000023490664,0.000016179716,0.00002443952],"domain_scores_gemma":[0.99913484,0.00023776121,0.000299358,0.00019557479,0.000054359214,0.00007819923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003861987,0.00038712923,0.00041795813,0.00085536455,0.00032679885,0.0012270643,0.00048391154,0.0008904711,0.001838618],"category_scores_gemma":[0.0030095892,0.00032119395,0.0003218232,0.0008285081,0.00079417246,0.0012786259,0.0005727076,0.0003156788,0.00043577657],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010321834,0.00009760548,0.8191522,0.00025537703,0.00029461362,0.0039993525,0.0013617412,0.021124752,0.06388861,0.046678018,0.0012279642,0.040887628],"study_design_scores_gemma":[0.00027849994,0.00042254405,0.63152975,0.00017310094,0.000350768,0.015369951,0.0017824022,0.17438619,0.042454105,0.12461069,0.008514896,0.00012722744],"about_ca_topic_score_codex":0.0012106542,"about_ca_topic_score_gemma":0.0017378399,"teacher_disagreement_score":0.001838618,"about_ca_system_score_codex":0.00029986896,"about_ca_system_score_gemma":0.00011925215,"threshold_uncertainty_score":0.006150782},"labels":[],"label_agreement":null},{"id":"W2009742384","doi":"10.1088/0004-637x/761/2/187","title":"A FIRST APPLICATION OF THE ALCOCK-PACZYNSKI TEST TO STACKED COSMIC VOIDS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Redshift; Galaxy; Astrophysics; Void (composites); Sky; Physics; COSMIC cancer database; Dark energy; Isotropy; Redshift survey; Astronomy; Cosmology; Optics; Materials science","score_opus":0.006348227400454514,"score_gpt":0.2125976044491228,"score_spread":0.20624937704866828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009742384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88711655,0.0004000349,0.09002641,0.0012334865,0.00033515808,0.00009937563,0.0007970187,0.0005837657,0.019408219],"genre_scores_gemma":[0.9933175,0.000051832987,0.0051867953,0.000113503804,0.000099887635,0.000026451413,0.0002759454,0.000060819773,0.000867256],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9983311,0.00038172683,0.000104359904,0.0005213499,0.0003536637,0.00030777397],"domain_scores_gemma":[0.9736217,0.01685892,0.0023911148,0.0034029414,0.001508342,0.0022168518],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028932518,0.0005884198,0.0012230462,0.0017537161,0.001636493,0.0020145357,0.002200646,0.0017204939,0.009998021],"category_scores_gemma":[0.036317065,0.0002906972,0.0013946347,0.0015485878,0.0024450913,0.0049455706,0.00409319,0.0018111711,0.00051954127],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020298911,0.0006226216,0.15417469,0.00056550896,0.00095244934,0.0023764286,0.0017905306,0.034239817,0.014283322,0.6310572,0.012022035,0.14588551],"study_design_scores_gemma":[0.0005008478,0.001059566,0.1283532,0.00012277573,0.00037007005,0.0015140241,0.0016430981,0.23353633,0.012808184,0.6073947,0.01237882,0.00031843354],"about_ca_topic_score_codex":0.0032108694,"about_ca_topic_score_gemma":0.0016380005,"teacher_disagreement_score":0.009998021,"about_ca_system_score_codex":0.0005361463,"about_ca_system_score_gemma":0.0007160062,"threshold_uncertainty_score":0.03344673},"labels":[],"label_agreement":null},{"id":"W2009743038","doi":"10.1088/0004-637x/769/1/80","title":"SEDS: THE SPITZER EXTENDED DEEP SURVEY. SURVEY DESIGN, PHOTOMETRY, AND DEEP IRAC SOURCE COUNTS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":286,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Western University","funders":"Science and Technology Facilities Council","keywords":"Physics; Cosmic variance; Chandra Deep Field South; Galaxy; Astrophysics; Photometry (optics); Hubble Deep Field; Cosmic infrared background; Redshift; COSMIC cancer database; Astronomy; Stars; Cosmic microwave background","score_opus":0.014509398264901715,"score_gpt":0.223024505571193,"score_spread":0.20851510730629128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009743038","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.041958116,0.0009431312,0.052908123,0.00072581484,0.00019578647,0.0025846392,0.8629362,0.014107097,0.023641195],"genre_scores_gemma":[0.054038048,0.00058296724,0.06296052,0.0005792048,0.00016520279,0.002528448,0.8650377,0.0027567693,0.011351049],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9985877,0.0003107648,0.00013457624,0.000223341,0.00060494343,0.00013856665],"domain_scores_gemma":[0.9962953,0.0003071182,0.0007617577,0.00070620247,0.0014705244,0.00045904546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0033707363,0.0011201686,0.0006464626,0.005242469,0.00052892184,0.0009962873,0.0017118289,0.0004430723,0.017891219],"category_scores_gemma":[0.0055807508,0.00057908933,0.00042975915,0.004640196,0.00037439994,0.00132303,0.001763207,0.0008505471,0.026676256],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004415981,0.00020129429,0.08603748,0.00045813122,0.000115024945,0.00012455977,0.00032099837,0.0033550763,0.0048955493,0.0044567045,0.75268143,0.14691211],"study_design_scores_gemma":[0.00030510902,0.00022293003,0.23006478,0.0002188973,0.000060892802,0.00028939228,0.00034147067,0.009349001,0.0030137142,0.00830596,0.7477355,0.00009236381],"about_ca_topic_score_codex":0.009296235,"about_ca_topic_score_gemma":0.009553816,"teacher_disagreement_score":0.017891219,"about_ca_system_score_codex":0.00093065295,"about_ca_system_score_gemma":0.0015536138,"threshold_uncertainty_score":0.059852123},"labels":[],"label_agreement":null},{"id":"W2009768899","doi":"10.1088/0004-637x/739/2/68","title":"PTF1 J071912.13+485834.0: AN OUTBURSTING AM CVn SYSTEM DISCOVERED BY A SYNOPTIC SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"White dwarf; Light curve; Photometry (optics); Orbital period; Cataclysmic variable star; Brightness; Accretion (finance); Dwarf nova","score_opus":0.03271020821612709,"score_gpt":0.23364981301363527,"score_spread":0.20093960479750816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009768899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99751174,0.000079393365,0.00018068752,0.000043222924,0.000010641948,0.000010673213,0.00047995648,0.000038010614,0.0016456657],"genre_scores_gemma":[0.99680966,0.00008202424,0.0006141853,0.00004977661,0.000041822153,0.000011786528,0.0018120506,0.000016583255,0.00056206604],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989164,0.000004267043,0.000004313975,0.00003844469,0.00002686909,0.00003456056],"domain_scores_gemma":[0.9996723,0.00002103688,0.000098833465,0.000027042612,0.000032918437,0.00014790379],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013665037,0.00022551997,0.00024456088,0.0013917682,0.00079993455,0.00038167028,0.00040304504,0.000323699,0.0013212571],"category_scores_gemma":[0.00023793569,0.00010657846,0.00013411185,0.0006444956,0.00024609204,0.0002555319,0.0006658264,0.00032963348,0.0002932087],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032007004,0.00019019398,0.90521234,0.00007366253,0.00004893127,0.005812694,0.0010664541,0.00040701035,0.046775773,0.0004596012,0.003915928,0.035717342],"study_design_scores_gemma":[0.00001028731,0.000067708155,0.99352914,0.0000073441047,0.000011702485,0.001977795,0.00014044448,0.0005413076,0.00083250453,0.00007982894,0.0027948853,0.000006981012],"about_ca_topic_score_codex":0.004723285,"about_ca_topic_score_gemma":0.009722887,"teacher_disagreement_score":0.004723285,"about_ca_system_score_codex":0.00037120137,"about_ca_system_score_gemma":0.00013160316,"threshold_uncertainty_score":0.009391606},"labels":[],"label_agreement":null},{"id":"W2009794476","doi":"10.1086/376603","title":"On the Use of Fractional Brownian Motion Simulations to Determine the Three‐dimensional Statistical Properties of Interstellar Gas","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Fractional Brownian motion; Centroid; Spectral density; Physics; Vector field; Brownian motion; Field (mathematics); Spectral index; Computational physics; Statistical physics; Geometry; Mechanics; Statistics; Spectral line; Mathematics; Quantum mechanics","score_opus":0.04142134636373728,"score_gpt":0.25895608253952546,"score_spread":0.21753473617578817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009794476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.72515863,0.00024337093,0.26830095,0.00043639497,0.00006656485,0.00009182822,0.00019438939,0.00036214938,0.005145732],"genre_scores_gemma":[0.95577186,0.00024309778,0.042715825,0.0000958373,0.000044584463,0.00015161818,0.00019419836,0.00010046373,0.00068257377],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998211,0.00007982998,0.00000926282,0.000021120588,0.00004034548,0.00002829656],"domain_scores_gemma":[0.99589217,0.0031294813,0.00029362933,0.00027069548,0.00023333273,0.00018077804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013869109,0.00070796616,0.0007716873,0.0009706245,0.0010139269,0.0010275308,0.0009609345,0.001138675,0.0011478667],"category_scores_gemma":[0.007019702,0.00037635976,0.00086886354,0.00067801535,0.0010924294,0.0010554685,0.0006510985,0.00091889815,0.00011848953],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024614275,0.000019785672,0.0011060708,0.000010686016,0.000020859148,0.00004321028,0.000039660303,0.9886614,0.00067079294,0.0081532635,0.00007548903,0.0011742658],"study_design_scores_gemma":[0.0000019078464,0.000002627177,0.000073837626,8.734441e-7,8.388327e-7,0.0000028502077,0.0000020099399,0.99912995,0.00005465728,0.0007086469,0.000019446119,0.00000229282],"about_ca_topic_score_codex":0.012010331,"about_ca_topic_score_gemma":0.0053674155,"teacher_disagreement_score":0.012010331,"about_ca_system_score_codex":0.00090588874,"about_ca_system_score_gemma":0.0006567069,"threshold_uncertainty_score":0.02388084},"labels":[],"label_agreement":null},{"id":"W2009844729","doi":"10.1086/503378","title":"Damping of Magnetohydrodynamic Turbulence in Solar Flares","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Solar flare; Electron; Computational physics; Landau damping; Particle acceleration; Magnetic damping; Magnetic field; Magnetohydrodynamics; Turbulence; Magnetic reconnection; Gyroradius; Plasma; Solar wind; Astrophysics; Mechanics; Nuclear physics","score_opus":0.0032678942877057628,"score_gpt":0.19973589632575356,"score_spread":0.1964680020380478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009844729","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9131905,0.0030955572,0.05838766,0.00044574344,0.00020023555,0.000094457035,0.00017796246,0.00045733576,0.023950648],"genre_scores_gemma":[0.99523455,0.00046118067,0.0022121381,0.000036389145,0.00005687128,0.000018931843,0.00006411936,0.000033450055,0.0018824561],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999659,0.0000046526206,0.000001962352,0.000003949321,0.000011792136,0.000011751923],"domain_scores_gemma":[0.99994326,0.000014367486,0.000017758592,0.0000039450533,0.0000085113825,0.000012195666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007044479,0.0005919275,0.00019459295,0.00030955186,0.00026874943,0.00045278436,0.00021757865,0.00032787674,0.0018818233],"category_scores_gemma":[0.00026454663,0.00008483676,0.00025845107,0.00014616903,0.00031413566,0.00024797863,0.0003991579,0.0002728189,0.00020374804],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043685103,0.00026105088,0.033372205,0.00029537868,0.00012362027,0.003385329,0.00076262536,0.4088299,0.3771573,0.1133858,0.0059605516,0.056029443],"study_design_scores_gemma":[0.00007150842,0.00032385305,0.058021963,0.00003206856,0.000020466181,0.001006758,0.00012061232,0.8851934,0.016235474,0.031429574,0.007495767,0.000048545076],"about_ca_topic_score_codex":0.0012582744,"about_ca_topic_score_gemma":0.0005660982,"teacher_disagreement_score":0.0018818233,"about_ca_system_score_codex":0.0003066641,"about_ca_system_score_gemma":0.00008566981,"threshold_uncertainty_score":0.006295383},"labels":[],"label_agreement":null},{"id":"W2009863857","doi":"10.1088/0004-637x/710/2/1239","title":"IONIZING RADIATION FROM<i>z</i>= 4–10 GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":128,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Reionization; Galaxy; Ionizing radiation; Background radiation; Population; Radiation; Dwarf galaxy; Star formation","score_opus":0.006066946079176734,"score_gpt":0.20368180902836,"score_spread":0.19761486294918326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009863857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99483514,0.00006322084,0.0020735417,0.00010169166,0.0000062670942,0.000008467434,0.00087255286,0.000095871445,0.001943317],"genre_scores_gemma":[0.99415696,0.00006353217,0.0031225125,0.00004221883,0.000009507816,0.000016731401,0.0019074625,0.000042209813,0.0006388459],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99990416,0.000018193321,0.0000052824444,0.000027863602,0.00001252815,0.000031973086],"domain_scores_gemma":[0.99932337,0.00030152407,0.00014520888,0.000064539185,0.00007103814,0.00009433417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002980522,0.000442303,0.00038313176,0.00043652556,0.00038864848,0.0006820091,0.001046023,0.0008581223,0.0018603206],"category_scores_gemma":[0.0021168403,0.00036728304,0.00065364176,0.00087891717,0.00061152445,0.00069734256,0.00049597706,0.00071569264,0.00022642985],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015700213,0.00006457502,0.05266186,0.000029388377,0.00008927831,0.00013230338,0.00006986108,0.9404793,0.00132796,0.0022686468,0.00051765336,0.0022022624],"study_design_scores_gemma":[0.00009731071,0.00008308556,0.028400421,0.000010690114,0.000046882848,0.00009890318,0.000095137315,0.9658679,0.0018119175,0.0025663862,0.0008945565,0.00002678871],"about_ca_topic_score_codex":0.023631606,"about_ca_topic_score_gemma":0.014378626,"teacher_disagreement_score":0.023631606,"about_ca_system_score_codex":0.0010050279,"about_ca_system_score_gemma":0.00043027583,"threshold_uncertainty_score":0.04698813},"labels":[],"label_agreement":null},{"id":"W2009877248","doi":"10.1086/421697","title":"Observation of M87 at 400 GeV with the Whipple 10 Meter Telescope","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Telescope; Galaxy; Flux (metallurgy); Astronomy; Sky; Cutoff; Sensitivity (control systems)","score_opus":0.010943152271832518,"score_gpt":0.20645853848686768,"score_spread":0.19551538621503517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009877248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99835026,0.000075065764,0.00027326043,0.000018498713,0.0000021621443,0.0000059832146,0.00033949857,0.000025513229,0.00090976525],"genre_scores_gemma":[0.99662966,0.00013597442,0.0011665372,0.000030271725,0.000012192381,0.000010615193,0.0014655052,0.000009188646,0.0005399965],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998387,0.00002262066,0.0000064818178,0.000024661791,0.0000558713,0.000051586245],"domain_scores_gemma":[0.9996137,0.00005042129,0.00016604668,0.000045505036,0.000041825446,0.00008259897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002639518,0.00026020678,0.00029369438,0.000997483,0.00036850214,0.0002366445,0.00034554576,0.00032055582,0.00058962364],"category_scores_gemma":[0.00042682953,0.0001658837,0.00017057698,0.00077282387,0.00020021516,0.00019057209,0.00056742656,0.000272014,0.0003536442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062506454,0.0001959396,0.915775,0.00005501027,0.00012252622,0.0021142215,0.0006999176,0.0014439347,0.05827851,0.00031263824,0.0019111468,0.018466128],"study_design_scores_gemma":[0.000012390569,0.00015435019,0.99447507,0.000006445029,0.000024721738,0.00058581826,0.0000803123,0.0007794523,0.0025253054,0.00006984477,0.0012796514,0.000006643817],"about_ca_topic_score_codex":0.0027762793,"about_ca_topic_score_gemma":0.010578381,"teacher_disagreement_score":0.0027762793,"about_ca_system_score_codex":0.00025481102,"about_ca_system_score_gemma":0.00015094619,"threshold_uncertainty_score":0.0055202246},"labels":[],"label_agreement":null},{"id":"W2009878614","doi":"10.1088/0004-637x/773/1/61","title":"A DEEP SEARCH FOR EXTENDED RADIO CONTINUUM EMISSION FROM DWARF SPHEROIDAL GALAXIES: IMPLICATIONS FOR PARTICLE DARK MATTER","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Astrophysics; Dark matter; WIMP; Astronomy; Galaxy; Surface brightness","score_opus":0.012108155950571022,"score_gpt":0.24970515313328545,"score_spread":0.23759699718271443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009878614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985689,0.000043975564,0.0005096942,0.000026334623,0.0000010170165,0.0000031137597,0.00015462226,0.000021560825,0.0006706788],"genre_scores_gemma":[0.9989618,0.000026096353,0.00061918725,0.000012054989,0.0000040237,0.000002230608,0.00021387021,0.000002322108,0.0001584016],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999434,0.000006020275,0.0000017679483,0.00001762431,0.000013097737,0.00001808317],"domain_scores_gemma":[0.99967706,0.000053193042,0.000090506066,0.00003979558,0.000023642227,0.00011590959],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013702172,0.00020829578,0.00012923231,0.0007047783,0.00021935023,0.00034497568,0.00023581451,0.0001733594,0.0006807772],"category_scores_gemma":[0.00026997676,0.00012213568,0.000117347125,0.0004372963,0.00022163078,0.00011861445,0.0003025139,0.00015786484,0.00015476234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013246064,0.00008236128,0.9205608,0.00003265378,0.00005157828,0.00038804498,0.0003697906,0.0010453102,0.05527158,0.00043971805,0.00038854047,0.021237167],"study_design_scores_gemma":[0.0000097531265,0.0000737885,0.99434304,0.0000047307194,0.000018293727,0.00026146826,0.000129889,0.0017981363,0.0024430316,0.000220171,0.0006932423,0.0000045067322],"about_ca_topic_score_codex":0.0024430417,"about_ca_topic_score_gemma":0.005558052,"teacher_disagreement_score":0.0024430417,"about_ca_system_score_codex":0.00015715352,"about_ca_system_score_gemma":0.00010952728,"threshold_uncertainty_score":0.0048575997},"labels":[],"label_agreement":null},{"id":"W2009922462","doi":"10.1088/0004-637x/758/2/74","title":"ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. I. THE INFLUENCE OF FEEDBACK, NON-THERMAL PRESSURE, AND CLUSTER SHAPES ON<i>Y</i>-<i>M</i>SCALING RELATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":239,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Intracluster medium; Astrophysics; Radiative cooling; Cluster (spacecraft); Redshift; Active galactic nucleus; Galaxy cluster; Sunyaev–Zel'dovich effect; Substructure; Scaling; Anisotropy; Halo; Galaxy; Geometry; Optics","score_opus":0.008011045579092558,"score_gpt":0.2114168317501402,"score_spread":0.20340578617104765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2009922462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9907912,0.00060203526,0.0021554253,0.00047577746,0.000014158823,0.00001933083,0.0011683009,0.00013476734,0.0046389727],"genre_scores_gemma":[0.99706405,0.00023568392,0.0013721826,0.00008878952,0.0000116849,0.000012615414,0.0008189162,0.000051970863,0.00034419374],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997756,0.00009230033,0.000008567462,0.000054992393,0.000034462395,0.00003415881],"domain_scores_gemma":[0.9989065,0.00053885614,0.00021856041,0.00011121543,0.00009304252,0.00013186091],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009485259,0.00037999247,0.0002868475,0.0007381137,0.00047812267,0.0007080562,0.0007665575,0.00045064342,0.0011160717],"category_scores_gemma":[0.0027758835,0.0002485638,0.00036619976,0.0009210615,0.00054558984,0.00068745273,0.0009074753,0.00035172483,0.000174199],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018742793,0.000057915135,0.6720684,0.00010612942,0.0002851739,0.0003091315,0.00045683386,0.29143944,0.0023337686,0.017527483,0.003954544,0.011273767],"study_design_scores_gemma":[0.00006643599,0.00007948163,0.58604974,0.000058615416,0.00004680467,0.0001392365,0.00026861747,0.39871535,0.0014589947,0.00831374,0.0047486913,0.00005429768],"about_ca_topic_score_codex":0.03940617,"about_ca_topic_score_gemma":0.042128928,"teacher_disagreement_score":0.03940617,"about_ca_system_score_codex":0.001360827,"about_ca_system_score_gemma":0.0004158518,"threshold_uncertainty_score":0.07835364},"labels":[],"label_agreement":null},{"id":"W2010065000","doi":"10.1088/0004-637x/750/2/94","title":"DISCOVERY OF HIGH-ENERGY AND VERY HIGH ENERGY γ-RAY EMISSION FROM THE BLAZAR RBS 0413","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Office of Science; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Centre National de la Recherche Scientifique; National Science Foundation; Agenzia Spaziale Italiana; Istituto Nazionale di Astrofisica; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; Science Foundation Ireland; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; U.S. Department of Energy; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution","keywords":"Blazar; Photon; Fermi Gamma-ray Space Telescope; Synchrotron; Spitzer Space Telescope; BL Lac object; Crab Nebula; Flux (metallurgy); Telescope","score_opus":0.00533312877664241,"score_gpt":0.18978879466501686,"score_spread":0.18445566588837445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010065000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975802,0.00022399148,0.0006149395,0.00003130997,0.000005244806,0.0000064285405,0.00022479847,0.00007588132,0.0012372427],"genre_scores_gemma":[0.9963271,0.0001886584,0.0019117375,0.00006038419,0.0000138492005,0.00000880648,0.0008377605,0.00003167533,0.00061992946],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999811,0.000019308862,0.000012120963,0.00004684705,0.00007246283,0.000038309285],"domain_scores_gemma":[0.9996394,0.00003873969,0.00016520306,0.00005238641,0.000043016826,0.00006127707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035509063,0.0003998452,0.00037468417,0.0006855897,0.00041447574,0.0008655735,0.00057826116,0.00037171927,0.00075414905],"category_scores_gemma":[0.00041783025,0.00029491834,0.00033214924,0.0006842806,0.0003214065,0.00012902558,0.00048046047,0.00038527444,0.00037740273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004363036,0.00014050769,0.75713986,0.00014346476,0.0002651355,0.0012794932,0.000516018,0.0020061517,0.2124973,0.0010797768,0.0011379804,0.023357982],"study_design_scores_gemma":[0.000027322161,0.00014636281,0.9810447,0.000020211817,0.000076890785,0.00081751955,0.00010503041,0.0022220747,0.011854451,0.00015868832,0.0035038164,0.000022970537],"about_ca_topic_score_codex":0.0044821845,"about_ca_topic_score_gemma":0.006648459,"teacher_disagreement_score":0.0044821845,"about_ca_system_score_codex":0.0004676634,"about_ca_system_score_gemma":0.00025164968,"threshold_uncertainty_score":0.008912206},"labels":[],"label_agreement":null},{"id":"W2010081861","doi":"10.1088/0004-637x/705/2/l223","title":"STAR STREAM FOLDING BY DARK GALACTIC SUBHALOS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics","funders":"","keywords":"Halo; Velocity dispersion; Stars; Dark matter; Dark matter halo; STREAMS; Galactic halo; Dispersion (optics)","score_opus":0.009503814944750435,"score_gpt":0.2655681368839462,"score_spread":0.25606432193919576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010081861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973507,0.000057355828,0.0011617929,0.000048027592,0.000010405969,0.000007761164,0.00009459615,0.000068844456,0.0012004906],"genre_scores_gemma":[0.99897754,0.00005451969,0.00042331222,0.000021048598,0.0000045218303,0.0000060093516,0.00011676733,0.000026773834,0.00036957918],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999944,0.000013227074,0.000003244335,0.000012362544,0.000007774439,0.000019522417],"domain_scores_gemma":[0.9996848,0.000066369415,0.000059089434,0.000043880893,0.00002774838,0.00011809127],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024699137,0.00029961436,0.00033588047,0.00031847102,0.0004141473,0.0008611267,0.00034595368,0.00036183972,0.0014820745],"category_scores_gemma":[0.0010418498,0.00020144507,0.0005546274,0.00026500432,0.0005141206,0.0005004408,0.0005865669,0.0003205616,0.00023883824],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058677804,0.00021878834,0.2364265,0.00009744052,0.00020771119,0.00079510285,0.0005295685,0.7242243,0.017313965,0.008099232,0.0012586835,0.010241899],"study_design_scores_gemma":[0.00010856832,0.00020100031,0.071082525,0.000025581801,0.00006529639,0.00010490008,0.00025953318,0.915298,0.005038262,0.005943547,0.0018362337,0.000036497688],"about_ca_topic_score_codex":0.0049960082,"about_ca_topic_score_gemma":0.0030173282,"teacher_disagreement_score":0.0049960082,"about_ca_system_score_codex":0.00057221483,"about_ca_system_score_gemma":0.00027180946,"threshold_uncertainty_score":0.009933829},"labels":[],"label_agreement":null},{"id":"W2010491283","doi":"10.1086/591489","title":"The Formation of Polar Disk Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy formation and evolution; Peculiar galaxy; Lenticular galaxy; Galaxy; Galaxy merger; Accretion (finance); Galaxy group; Galaxy rotation curve; Angular momentum; Polar; Elliptical galaxy; Classical mechanics","score_opus":0.007820951654983197,"score_gpt":0.20172713704002243,"score_spread":0.19390618538503923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010491283","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9731609,0.00081706716,0.0051274165,0.0004883313,0.000042947915,0.000020267878,0.00018683572,0.00007356325,0.020082673],"genre_scores_gemma":[0.9987036,0.0001784985,0.00048818585,0.00003369777,0.00000763623,0.0000032336486,0.00006912,0.000005053434,0.0005109254],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998517,0.000045100544,0.000004184168,0.00004385772,0.000022195867,0.000033021068],"domain_scores_gemma":[0.9996476,0.000073815885,0.0000889724,0.000049453865,0.0000241069,0.000115979485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031509995,0.00022038876,0.00022856421,0.0002811878,0.00056375406,0.0018757997,0.0003775591,0.0006698393,0.0019114164],"category_scores_gemma":[0.0017972728,0.00031957112,0.00024837925,0.00018186079,0.0011391361,0.0010688346,0.0009464262,0.00041583017,0.00043050232],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058046414,0.00016610809,0.47199646,0.00020072906,0.00015111001,0.0012831335,0.002417375,0.1317514,0.028302517,0.31651464,0.006879152,0.03975699],"study_design_scores_gemma":[0.00041068761,0.0004812638,0.47241858,0.00018720167,0.00020815892,0.0022802223,0.0029961267,0.2844061,0.015699426,0.17029953,0.0504179,0.00019488703],"about_ca_topic_score_codex":0.004314305,"about_ca_topic_score_gemma":0.0021758697,"teacher_disagreement_score":0.004314305,"about_ca_system_score_codex":0.00080841826,"about_ca_system_score_gemma":0.00033092164,"threshold_uncertainty_score":0.00857836},"labels":[],"label_agreement":null},{"id":"W2010588984","doi":"10.1086/422462","title":"Velocity Modification of the Power Spectrum from an Absorbing Medium","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":152,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Spectral density; Computational physics; Turbulence; Physics; Intensity (physics); Spectral line; Line (geometry); Scaling; Spectral index; Absorption (acoustics); Scale (ratio); Radiant intensity; Energy (signal processing); Range (aeronautics); Statistical physics; Optics; Statistics; Mechanics; Materials science; Mathematics; Quantum mechanics; Geometry","score_opus":0.010982894021959065,"score_gpt":0.25741848883233237,"score_spread":0.2464355948103733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010588984","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2872338,0.0002039277,0.7072756,0.0001295492,0.00004160587,0.00002308732,0.0002720132,0.00035761765,0.0044627604],"genre_scores_gemma":[0.96566486,0.00030439193,0.031132935,0.000043603442,0.00006127166,0.0000349168,0.00024539934,0.00009537792,0.0024172098],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986196,0.000026592117,0.0000064384476,0.00003230995,0.00004811731,0.000024518466],"domain_scores_gemma":[0.99896955,0.00045465285,0.00024857218,0.00012876192,0.00012432008,0.0000742066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042161954,0.00040098457,0.00021327153,0.00083691924,0.0002048494,0.0010624263,0.00050014135,0.00021461233,0.0010722965],"category_scores_gemma":[0.0020357564,0.00017912957,0.00025472333,0.00050479354,0.0008105707,0.0011563716,0.0005445648,0.00059099426,0.00014813253],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016362948,0.00008946791,0.010037544,0.00014002138,0.00006420858,0.0007545894,0.00033065316,0.33283833,0.17747615,0.43926612,0.0009737256,0.037865542],"study_design_scores_gemma":[0.0000027785459,0.00003640953,0.0049628317,0.0000091358115,0.000008595103,0.00014406003,0.000027051125,0.955408,0.0062209135,0.03238663,0.00076847593,0.00002522363],"about_ca_topic_score_codex":0.0012844403,"about_ca_topic_score_gemma":0.0007536415,"teacher_disagreement_score":0.0012844403,"about_ca_system_score_codex":0.00043083567,"about_ca_system_score_gemma":0.00034543214,"threshold_uncertainty_score":0.0035871863},"labels":[],"label_agreement":null},{"id":"W2010603369","doi":"10.1088/0004-637x/691/2/l63","title":"AN ALTERNATIVE ORIGIN FOR HYPERVELOCITY STARS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Milky Way; Supermassive black hole; Dwarf galaxy; Stars; Galaxy; Star cluster; Halo; Globular cluster; Stellar dynamics","score_opus":0.02498351415195671,"score_gpt":0.28427149812765945,"score_spread":0.25928798397570274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010603369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88405883,0.0035165995,0.035001606,0.002021421,0.00026841825,0.000037815676,0.00038142578,0.00038376934,0.07433004],"genre_scores_gemma":[0.9863405,0.00041645975,0.0025944002,0.00031695067,0.00008250469,0.000011166019,0.00019087164,0.000025235493,0.010021859],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997683,0.000020279293,0.0000071515205,0.00008926643,0.00003549517,0.00007943861],"domain_scores_gemma":[0.99957615,0.000053649983,0.000077801706,0.0000873991,0.00007771605,0.0001272774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024252193,0.00027432098,0.00030005458,0.00046387684,0.0006585546,0.0020355452,0.00092717604,0.0012223562,0.007562332],"category_scores_gemma":[0.00080472743,0.0001900279,0.00030216944,0.00050277554,0.00088781555,0.0014790398,0.0013454868,0.00065305864,0.0015842378],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003642675,0.00012437635,0.20152609,0.00029718215,0.0001434619,0.0035837681,0.002803743,0.0047549168,0.040295772,0.6776029,0.006205036,0.062298506],"study_design_scores_gemma":[0.0003283539,0.00041134327,0.24854094,0.000401631,0.00014888989,0.011981933,0.0049624313,0.04543305,0.025994318,0.36854106,0.293058,0.00019802662],"about_ca_topic_score_codex":0.0010947078,"about_ca_topic_score_gemma":0.0014553505,"teacher_disagreement_score":0.007562332,"about_ca_system_score_codex":0.0006160259,"about_ca_system_score_gemma":0.0003216137,"threshold_uncertainty_score":0.025298536},"labels":[],"label_agreement":null},{"id":"W2010633662","doi":"10.1086/321358","title":"Gas, Dust, and Young Stars in the Outer Disk of M31","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Stars; Galaxy; Star formation; Dust lane; Astronomy; Extinction (optical mineralogy); Photometry (optics); Interstellar medium; Molecular cloud; Thick disk; Population; Halo","score_opus":0.007354804440543281,"score_gpt":0.2093604348258672,"score_spread":0.2020056303853239,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010633662","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99978346,0.000050969105,0.000021989526,0.000006700705,2.9439917e-7,0.0000012308219,0.000029841452,0.0000013848498,0.00010419346],"genre_scores_gemma":[0.999193,0.000088043,0.00022642095,0.0000079115025,0.0000019896029,0.0000023082064,0.0002596033,0.000001585817,0.00021919158],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990785,0.000010979213,0.00000662299,0.000023467328,0.00002174276,0.000029347286],"domain_scores_gemma":[0.99959236,0.00004152623,0.000121910445,0.000047209014,0.00007357608,0.00012353079],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017852952,0.00020939499,0.00019858294,0.0006487058,0.00066370936,0.00045643488,0.00027969264,0.0002284228,0.00045900152],"category_scores_gemma":[0.0006733259,0.00023825963,0.00009716635,0.0006161612,0.00042474634,0.00041425927,0.00050510356,0.00016196564,0.00019003624],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023193777,0.000091090194,0.9197412,0.000038156522,0.00003489206,0.00083647075,0.0019181841,0.0012195722,0.06832268,0.00019082538,0.0001522956,0.007222739],"study_design_scores_gemma":[0.0000067570877,0.000056616827,0.997013,0.000005280982,0.0000062925524,0.00025803587,0.00027109086,0.00058904005,0.001271832,0.000060376165,0.0004561626,0.0000054936986],"about_ca_topic_score_codex":0.045124166,"about_ca_topic_score_gemma":0.07364427,"teacher_disagreement_score":0.045124166,"about_ca_system_score_codex":0.0006178702,"about_ca_system_score_gemma":0.00035187727,"threshold_uncertainty_score":0.08972305},"labels":[],"label_agreement":null},{"id":"W2010672216","doi":"10.1086/425992","title":"Neutrino Emission and Mass Ejection in Quark Novae","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Calgary","funders":"","keywords":"Neutrino; Strange matter; Measurements of neutrino speed; Solar neutrino problem; Quark; Nova (rocket); Core (optical fiber); Neutrino oscillation","score_opus":0.008718092424752152,"score_gpt":0.22806818806236334,"score_spread":0.21935009563761118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010672216","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968815,0.00034368306,0.0009632934,0.00004443744,0.000007296898,0.000002723951,0.0000141129985,0.000010904318,0.0017320161],"genre_scores_gemma":[0.9989342,0.00016865028,0.0003533506,0.000017682649,0.0000056962363,0.0000022346858,0.00002901156,0.0000045411934,0.00048448707],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999336,0.00001910863,0.0000030882734,0.000010150017,0.000011356969,0.000022711025],"domain_scores_gemma":[0.9996773,0.0001366459,0.0000805971,0.000022060178,0.000016983126,0.000066426604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027887174,0.00027884595,0.00023599491,0.00038511175,0.0005355592,0.0006774505,0.00019849834,0.0005557728,0.0008317913],"category_scores_gemma":[0.00094213075,0.00017010923,0.0002219065,0.00032873874,0.00041003214,0.00029859404,0.0007742616,0.00042614303,0.00014920138],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028698246,0.00057233905,0.50845003,0.00016384001,0.00019292823,0.011194473,0.0013835509,0.029055687,0.38009045,0.028842192,0.00078331225,0.036401477],"study_design_scores_gemma":[0.00024670362,0.001186112,0.7019581,0.000071666414,0.00014110238,0.008678902,0.0012952186,0.13670291,0.09924244,0.044054892,0.0063179927,0.00010398335],"about_ca_topic_score_codex":0.0010404394,"about_ca_topic_score_gemma":0.0008047316,"teacher_disagreement_score":0.0010404394,"about_ca_system_score_codex":0.0002557561,"about_ca_system_score_gemma":0.00007714434,"threshold_uncertainty_score":0.0027825832},"labels":[],"label_agreement":null},{"id":"W2010674535","doi":"10.1088/0004-637x/724/2/946","title":"FARADAY ROTATION IN THE TAIL OF THE PLANETARY NEBULA DeHt 5","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan College; Herzberg Institute of Astrophysics","funders":"","keywords":"Interstellar medium; Nebula; Magnetic field; Planetary nebula; Polarization (electrochemistry); Faraday effect; Stars; Solar rotation; Electron density","score_opus":0.006566662630126702,"score_gpt":0.21593294245170344,"score_spread":0.20936627982157674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010674535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974668,0.000096306656,0.00030111577,0.000023296701,0.0000050681188,0.000002215468,0.0001454728,0.000026643878,0.0019329159],"genre_scores_gemma":[0.9993218,0.00004296045,0.00019801575,0.000012522645,0.0000052569603,0.0000011126708,0.00021181925,0.0000028251143,0.0002037271],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999776,0.0000013558756,7.8039125e-7,0.000007100967,0.000004741854,0.000008328541],"domain_scores_gemma":[0.99992335,0.000014399983,0.000019746518,0.0000063401667,0.000010697894,0.000025367997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000052775937,0.00010458286,0.00008317459,0.00036305806,0.0002040453,0.00027437462,0.00010367107,0.00017920166,0.0008378537],"category_scores_gemma":[0.00016046946,0.00009937062,0.000081490885,0.00021461438,0.00011722309,0.00017107086,0.0002554985,0.00017521567,0.00012883256],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058147736,0.0000801839,0.78506684,0.00006861731,0.000071739625,0.0019224728,0.0006275328,0.0043705734,0.16733506,0.00065204315,0.001470191,0.03775333],"study_design_scores_gemma":[0.0000066777097,0.0000449837,0.9935486,0.0000060649045,0.000009540634,0.00040855582,0.00009666725,0.0019431125,0.0022728336,0.0001231864,0.0015345498,0.0000052264695],"about_ca_topic_score_codex":0.0020618672,"about_ca_topic_score_gemma":0.0033904745,"teacher_disagreement_score":0.0020618672,"about_ca_system_score_codex":0.00015995966,"about_ca_system_score_gemma":0.0000525513,"threshold_uncertainty_score":0.004099667},"labels":[],"label_agreement":null},{"id":"W2010718885","doi":"10.1086/519545","title":"A Three‐Stage Model for the Inner Engine of Gamma‐Ray Bursts: Prompt Emission and Early Afterglow","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Afterglow; Physics; Gamma-ray burst; Astrophysics; Neutron star; Ejecta; Supernova; Black hole (networking); Stage (stratigraphy); Context (archaeology); Astronomy; Accretion (finance); Jet (fluid)","score_opus":0.012585228691734842,"score_gpt":0.23828781978208324,"score_spread":0.2257025910903484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010718885","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22878966,0.0030177445,0.65942466,0.008779436,0.0008886217,0.00044826863,0.000683754,0.0015069122,0.09646094],"genre_scores_gemma":[0.9101369,0.0016150338,0.048158497,0.00076936575,0.00048375299,0.00047227877,0.00032009647,0.00018898475,0.03785504],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997564,0.00004526731,0.0000155097,0.000044822693,0.000052515505,0.00008550226],"domain_scores_gemma":[0.9993333,0.00021259395,0.000116566545,0.000065258704,0.000121215584,0.00015103891],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007649347,0.0010256168,0.0008107036,0.0006782034,0.0007967747,0.0020239903,0.003095178,0.0026923951,0.008308726],"category_scores_gemma":[0.0010680142,0.0006480637,0.0018272375,0.00043089275,0.0012700617,0.0036965774,0.0013664393,0.0010232959,0.0025307802],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034450373,0.00023329447,0.009660695,0.00030342853,0.00013743217,0.0028061133,0.00095247384,0.21964985,0.015348353,0.7284533,0.005151417,0.016959203],"study_design_scores_gemma":[0.00020672959,0.00025174985,0.0025314116,0.000038604696,0.00008367572,0.00089447905,0.00012389229,0.6570139,0.0013791695,0.32933378,0.0080494555,0.00009317046],"about_ca_topic_score_codex":0.0033384045,"about_ca_topic_score_gemma":0.0020693059,"teacher_disagreement_score":0.008308726,"about_ca_system_score_codex":0.00079343986,"about_ca_system_score_gemma":0.001167455,"threshold_uncertainty_score":0.027795494},"labels":[],"label_agreement":null},{"id":"W2010760843","doi":"10.1086/430341","title":"A Cool Magnetized Shell Wrapped around the Hot H<scp>ii</scp>Region S106: Geometry, Kinematics, Magnetic Vectors, and Pressure Balance","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; James Clerk Maxwell Telescope; Nebula; Bipolar outflow; Magnetic field; Outflow; Submillimeter Array; Shell (structure); Ionization; Ram pressure; Molecular cloud; Magnetohydrodynamics; H II region; Millimeter; Polarization (electrochemistry); Turbulence; Stars; Star formation; Ion; Mechanics","score_opus":0.0077564858506034,"score_gpt":0.21445210732721098,"score_spread":0.20669562147660758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010760843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97943443,0.00015592795,0.0019170439,0.00032900381,0.00010074235,0.000027506803,0.00038486495,0.00030796303,0.017342461],"genre_scores_gemma":[0.99751127,0.0000160174,0.0006848843,0.00005295241,0.000029379873,0.0000026265855,0.00020842443,0.000023219063,0.0014713192],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993587,0.0000075309667,0.000002504885,0.000022156664,0.000017779337,0.000014175585],"domain_scores_gemma":[0.9997348,0.000024880283,0.00007703324,0.00003025187,0.000026195345,0.000106864616],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000104310464,0.00023058431,0.0002994687,0.0002506502,0.00060507806,0.000610341,0.00035498923,0.0003848154,0.004110019],"category_scores_gemma":[0.00039313064,0.00022727362,0.00015449163,0.00019504788,0.00046675085,0.00026035245,0.00071615557,0.00026462862,0.0005995467],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024988684,0.0001464282,0.18195374,0.00029400428,0.00014886096,0.012047215,0.0011744744,0.012332836,0.73313713,0.008544471,0.011190028,0.036532044],"study_design_scores_gemma":[0.00024191543,0.0009900765,0.9266262,0.00003013385,0.0000588283,0.0047596837,0.00069145084,0.011659652,0.03749295,0.002526622,0.014857107,0.000065272114],"about_ca_topic_score_codex":0.0011266544,"about_ca_topic_score_gemma":0.00089700427,"teacher_disagreement_score":0.004110019,"about_ca_system_score_codex":0.00023175668,"about_ca_system_score_gemma":0.0001872351,"threshold_uncertainty_score":0.013749361},"labels":[],"label_agreement":null},{"id":"W2010764950","doi":"10.1086/587983","title":"Spectra of Carbon Nanoparticles: Laboratory Simulation of the Aromatic CH Emission Feature at 3.29 μm","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Carbon Nanotubes in Composites","field":"Materials Science","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Polycyclic aromatic hydrocarbon; Carbon fibers; Hydrocarbon; Amorphous carbon; Spectral line; Physics; Absorption (acoustics); Interstellar medium; Side chain; Molecule; Carbon Nanoparticles; Nanoparticle; Amorphous solid; Analytical Chemistry (journal); Astrophysics; Chemistry; Materials science; Organic chemistry; Astrobiology; Nuclear magnetic resonance; Composite number; Astronomy; Optics; Polymer; Composite material","score_opus":0.009023905882027864,"score_gpt":0.23202162603508705,"score_spread":0.2229977201530592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010764950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915245,0.00006956434,0.0026693922,0.00013488511,0.000014483244,0.000011101151,0.00021715307,0.00015362332,0.0052052736],"genre_scores_gemma":[0.9986985,0.00002557417,0.0006539703,0.000017882532,0.0000021452277,0.000008655811,0.00012974512,0.000016170583,0.0004472574],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999946,0.000005459375,0.0000014312596,0.0000129542805,0.0000188218,0.000015333555],"domain_scores_gemma":[0.9997789,0.000095727184,0.000023943576,0.000014930388,0.000058897567,0.000027550688],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014371028,0.00021524722,0.0001781488,0.00018456834,0.00027228854,0.00024602283,0.00044731988,0.00052883587,0.00239679],"category_scores_gemma":[0.00037063882,0.00009984602,0.00030283307,0.00016730413,0.00029800646,0.0002625498,0.00016244726,0.00044371307,0.00017385354],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068858505,0.0005099814,0.010569601,0.00018902835,0.00008014933,0.001395373,0.00031372337,0.58552176,0.3851702,0.0038502729,0.0025264823,0.009184852],"study_design_scores_gemma":[0.000089935085,0.00041282846,0.012223132,0.000012157504,0.000024391546,0.00016243075,0.00017522232,0.8429933,0.14185427,0.00089795655,0.0011142164,0.000040147726],"about_ca_topic_score_codex":0.0052699135,"about_ca_topic_score_gemma":0.0021556376,"teacher_disagreement_score":0.0052699135,"about_ca_system_score_codex":0.0008462713,"about_ca_system_score_gemma":0.00022503259,"threshold_uncertainty_score":0.010478497},"labels":[],"label_agreement":null},{"id":"W2010884090","doi":"10.1086/508509","title":"Iron in Hot DA White Dwarfs","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; University of Victoria","funders":"","keywords":"White dwarf; Astrophysics; Physics; Ultraviolet; Spectrograph; Spectral line; Spectroscopy; Very Large Telescope; Accretion (finance); Space Telescope Imaging Spectrograph; Astronomy; Abundance (ecology); Stars; Hubble space telescope; Optics","score_opus":0.008341246651407369,"score_gpt":0.21408785424999063,"score_spread":0.20574660759858326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010884090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997396,0.00009069958,0.00003764522,0.0000023626158,5.7559913e-7,6.7453453e-7,0.000025572794,0.0000015231575,0.00010136601],"genre_scores_gemma":[0.9995295,0.000061177896,0.000077733624,0.0000073974197,0.0000040625036,0.000001027633,0.0001276797,0.000001588866,0.00018990919],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989927,0.000010203241,0.0000073567826,0.000033668883,0.000024314584,0.000025154666],"domain_scores_gemma":[0.999785,0.000024030627,0.00007520633,0.000016458742,0.00003520315,0.00006416809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011954567,0.00017158905,0.00025370583,0.0010332862,0.0003986571,0.00033209793,0.0001781724,0.00018671613,0.0003754715],"category_scores_gemma":[0.0002676476,0.00011375776,0.00010329638,0.00052629394,0.0003347943,0.00016852705,0.00029798714,0.00011558754,0.00014339598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003058517,0.0000590596,0.9033901,0.00003287613,0.000050204366,0.0005966674,0.000862823,0.00011081185,0.087988645,0.000109379114,0.00009137485,0.0064022136],"study_design_scores_gemma":[0.0000032538385,0.00008782117,0.99586606,0.0000022374202,0.000010532206,0.00077082135,0.00021260764,0.000086325505,0.0025902693,0.000050808536,0.000317218,0.0000020562939],"about_ca_topic_score_codex":0.002262403,"about_ca_topic_score_gemma":0.003987562,"teacher_disagreement_score":0.002262403,"about_ca_system_score_codex":0.00015525393,"about_ca_system_score_gemma":0.00006982408,"threshold_uncertainty_score":0.0044984818},"labels":[],"label_agreement":null},{"id":"W2010893298","doi":"10.1088/0004-637x/761/2/155","title":"THE YOUNG OPEN CLUSTERS KING 12, NGC 7788, AND NGC 7790: PRE-MAIN-SEQUENCE STARS AND EXTENDED STELLAR HALOS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Stars; Halo; Hubble sequence; Astronomy; Open cluster; Main sequence; Star cluster; Luminosity; Blue straggler; Galaxy; Spiral galaxy","score_opus":0.0200605486336661,"score_gpt":0.25778144616508264,"score_spread":0.23772089753141654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010893298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99927276,0.00005692299,0.000048564576,0.0000029832509,4.7890643e-7,0.0000014439051,0.00008310959,0.00000477892,0.000528978],"genre_scores_gemma":[0.99929965,0.000037577873,0.00012672122,0.0000027346578,8.552589e-7,0.0000023882337,0.00025452868,0.000002629067,0.0002729291],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991953,0.0000030647466,0.0000047254175,0.000019900028,0.000021675005,0.000030993015],"domain_scores_gemma":[0.9995167,0.00005067748,0.00016942799,0.00003826154,0.000064694956,0.00016021961],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008989158,0.00016022206,0.00018869361,0.0009210044,0.00032425806,0.00039761755,0.0003153479,0.00016095921,0.00094773143],"category_scores_gemma":[0.00032832063,0.00013339736,0.000119904944,0.0005944737,0.0003213878,0.0003026039,0.0007379776,0.00012498735,0.00026310483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066727086,0.00005385905,0.94964904,0.00005901437,0.000037910042,0.0004022729,0.0011302263,0.0008582448,0.033636954,0.0007672473,0.00030329466,0.012434689],"study_design_scores_gemma":[0.000005687844,0.00003231517,0.9978429,0.0000030341705,0.000007668698,0.00013798269,0.00036628763,0.00025638708,0.00085238536,0.000071188115,0.0004194117,0.0000047204044],"about_ca_topic_score_codex":0.0147287585,"about_ca_topic_score_gemma":0.030572725,"teacher_disagreement_score":0.0147287585,"about_ca_system_score_codex":0.00055857765,"about_ca_system_score_gemma":0.0002015246,"threshold_uncertainty_score":0.029286027},"labels":[],"label_agreement":null},{"id":"W2010933530","doi":"10.1086/317823","title":"A Broadband X‐Ray Study of Supernova Remnant 3C 397","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"ROSAT; Supernova remnant; Ionization; Supernova; Emission spectrum; Cosmic ray; Spectral line","score_opus":0.009100252638240587,"score_gpt":0.2255686821240975,"score_spread":0.21646842948585693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2010933530","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99744606,0.00009270391,0.00012312456,0.000011779777,0.0000017624704,0.00000841633,0.00025740897,0.000016523067,0.0020423317],"genre_scores_gemma":[0.9973463,0.00018630744,0.0004859935,0.00002728395,0.000009397131,0.000009380737,0.0012348623,0.000021374935,0.00067907874],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.000003511534,0.0000035496894,0.000016746188,0.00001980889,0.000018962512],"domain_scores_gemma":[0.9998628,0.000018400031,0.00003078054,0.000020730135,0.000029357327,0.000038008166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013204777,0.00037294405,0.0003889878,0.0008680592,0.0007582335,0.00031733417,0.00036002294,0.0003560365,0.0013234087],"category_scores_gemma":[0.00014651522,0.00015875985,0.00038656074,0.0006155956,0.0002218037,0.00023339875,0.00043122377,0.0002753471,0.0005683825],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012979176,0.00047636058,0.3419828,0.00018682216,0.00018578985,0.011966884,0.00094840064,0.0036392873,0.61759895,0.0015717037,0.0009178732,0.019227229],"study_design_scores_gemma":[0.0000301698,0.000592282,0.9613894,0.000031961226,0.000066636174,0.0066672317,0.00056046224,0.0041121934,0.020114824,0.00037956727,0.0060167885,0.000038411494],"about_ca_topic_score_codex":0.0069308197,"about_ca_topic_score_gemma":0.007071398,"teacher_disagreement_score":0.0069308197,"about_ca_system_score_codex":0.00042019272,"about_ca_system_score_gemma":0.00014807844,"threshold_uncertainty_score":0.0137809515},"labels":[],"label_agreement":null},{"id":"W2011004962","doi":"10.1086/381049","title":"Constraints on QSO Models from a Relation between the QSO Luminosity Function and the Local Black Hole Mass Function","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"QSOS; Accretion (finance); Galaxy; Quasar; Luminosity function; Luminosity; Eddington luminosity; Black hole (networking)","score_opus":0.01032841406841299,"score_gpt":0.19438244580781375,"score_spread":0.18405403173940077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011004962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93105346,0.0011200553,0.060306642,0.00047636862,0.000016079297,0.000028169601,0.00063466193,0.00020686779,0.006157729],"genre_scores_gemma":[0.9969326,0.0002264048,0.0022026296,0.000036181744,0.000034611207,0.000009403936,0.00034576395,0.000034206536,0.00017825965],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99953425,0.00014086335,0.000036700665,0.00012215541,0.00008904872,0.00007703291],"domain_scores_gemma":[0.99373347,0.0035736004,0.0012819951,0.0007586897,0.00030316648,0.00034911206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020660795,0.0007014554,0.0006864926,0.0013278888,0.00043494257,0.001808517,0.0007823275,0.000562855,0.0017437082],"category_scores_gemma":[0.009306746,0.00035657967,0.00064611057,0.0007500852,0.00080429553,0.0018886018,0.0008647998,0.00047399732,0.00043678572],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039794232,0.0001123161,0.6989887,0.0002070373,0.00033701674,0.00082144677,0.0010423593,0.1571449,0.023279259,0.07034759,0.0014203055,0.04590117],"study_design_scores_gemma":[0.000051068822,0.00008062277,0.41298556,0.00008351307,0.00014479598,0.00045003335,0.00035806737,0.531042,0.0028855016,0.04908654,0.0027440747,0.00008828884],"about_ca_topic_score_codex":0.005746698,"about_ca_topic_score_gemma":0.0043472727,"teacher_disagreement_score":0.005746698,"about_ca_system_score_codex":0.0009444899,"about_ca_system_score_gemma":0.00035085945,"threshold_uncertainty_score":0.011426508},"labels":[],"label_agreement":null},{"id":"W2011044354","doi":"10.1088/0004-637x/778/2/88","title":"LONG-TERM EVOLUTION OF DECAYING MAGNETOHYDRODYNAMIC TURBULENCE IN THE MULTIPHASE INTERSTELLAR MEDIUM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Magnetohydrodynamics; Turbulence; Magnetohydrodynamic turbulence; Interstellar medium; Magnetic field; Magnetohydrodynamic drive; Kinetic energy; Compressibility; Supersonic speed","score_opus":0.007403662796527181,"score_gpt":0.23293742309561874,"score_spread":0.22553376029909156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011044354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984438,0.000044876517,0.00093699567,0.000035129444,0.000005109991,0.000004754526,0.000042049654,0.0000310519,0.00045621383],"genre_scores_gemma":[0.9994937,0.000024291447,0.00026207755,0.0000062859535,0.0000019048953,0.0000034719862,0.00007660818,0.000009035818,0.0001224591],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999374,0.000009769074,0.0000043531786,0.0000137686675,0.000011806103,0.000022783242],"domain_scores_gemma":[0.99959034,0.000093425624,0.00009193624,0.000034619017,0.000056870365,0.00013275877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026821165,0.00036078983,0.00030426934,0.00041744212,0.00048134907,0.00080483063,0.00037896438,0.0004293744,0.00040950344],"category_scores_gemma":[0.001015822,0.00023709101,0.00040832948,0.00027951776,0.00066935585,0.00066411047,0.00051779806,0.00056136743,0.000076045675],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010123457,0.00075480517,0.131839,0.000107052816,0.00024693043,0.0022484753,0.00062781107,0.6188467,0.21920826,0.013399487,0.0008614676,0.010847702],"study_design_scores_gemma":[0.000057504167,0.00020479111,0.051641192,0.000011421808,0.000028762934,0.00010822726,0.000116765616,0.9346196,0.011629741,0.0012959922,0.0002398044,0.00004616344],"about_ca_topic_score_codex":0.004043059,"about_ca_topic_score_gemma":0.001572415,"teacher_disagreement_score":0.004043059,"about_ca_system_score_codex":0.00072940043,"about_ca_system_score_gemma":0.00035062776,"threshold_uncertainty_score":0.008039057},"labels":[],"label_agreement":null},{"id":"W2011059721","doi":"10.1086/319120","title":"Discovery of Five Binary Radio Pulsars","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Galactic plane; Binary number; Binary pulsar; White dwarf; Astronomy; Orbital elements; Spin (aerodynamics); Millisecond pulsar; Stars; Mathematics","score_opus":0.011058139149325286,"score_gpt":0.3025594990366127,"score_spread":0.2915013598872874,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011059721","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969702,0.00086625194,0.00065980176,0.00007950736,0.000055587614,0.000012068267,0.00009185052,0.000018210969,0.0012466251],"genre_scores_gemma":[0.99802893,0.00026000213,0.00067273783,0.000114046416,0.00003324474,0.000008484294,0.00034413819,0.0000030233027,0.0005353681],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958783,0.00004176163,0.000046623663,0.000105818006,0.000087098655,0.00013089753],"domain_scores_gemma":[0.99915385,0.00016504362,0.00027158283,0.00007244187,0.00006726629,0.000269754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031355457,0.00024385609,0.00035256814,0.0010417209,0.0009476479,0.0013189631,0.00038846993,0.0005297516,0.00189719],"category_scores_gemma":[0.0018775665,0.00024289197,0.00019463712,0.0004926501,0.000548514,0.00028202115,0.0010034546,0.00041391898,0.00042067745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006603777,0.00021575384,0.898981,0.00017492735,0.00010338328,0.012872407,0.0013779207,0.000121396035,0.018851727,0.0017401414,0.0009620753,0.0639389],"study_design_scores_gemma":[0.000110089415,0.002289205,0.90725404,0.00011287253,0.0002632451,0.03945615,0.0013205099,0.00048002653,0.014463331,0.0009934866,0.03320087,0.000056124023],"about_ca_topic_score_codex":0.00091152784,"about_ca_topic_score_gemma":0.00092125277,"teacher_disagreement_score":0.00189719,"about_ca_system_score_codex":0.00028190046,"about_ca_system_score_gemma":0.00014354169,"threshold_uncertainty_score":0.0063467026},"labels":[],"label_agreement":null},{"id":"W2011087021","doi":"10.1086/496918","title":"The Population of <i>B</i> <i>z</i> <i>K</i> -selected ULIRGs at <i>z</i> ~ 2","year":2005,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":168,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Stellar mass; Luminous infrared galaxy; Star (game theory); Astronomy","score_opus":0.005033983586986738,"score_gpt":0.20083734875270468,"score_spread":0.19580336516571795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011087021","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99926335,0.0000353512,0.000042593245,0.0000095105825,5.675722e-7,0.0000035571784,0.0002252319,0.000008144473,0.00041163433],"genre_scores_gemma":[0.99856514,0.000030321375,0.00007563745,0.00001791985,0.0000026940409,0.0000056669637,0.0010033053,0.0000035295502,0.000295638],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979216,0.000010679082,0.000007629681,0.00007015763,0.000029471834,0.00008997514],"domain_scores_gemma":[0.99969435,0.000021823305,0.00010321973,0.000026887576,0.00003452321,0.00011922287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020776679,0.00020844796,0.00024099485,0.0013014624,0.00034222822,0.00071074924,0.0004929181,0.00029611203,0.0017552025],"category_scores_gemma":[0.000352949,0.00014837088,0.00016433708,0.0006910968,0.0003626065,0.00038437432,0.00047847556,0.00020783019,0.0006742895],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016605252,0.00006309535,0.9904856,0.000010852567,0.000025695046,0.00008163813,0.00038041783,0.00010057321,0.0049229492,0.00015112766,0.0002652199,0.0033467896],"study_design_scores_gemma":[0.000005453035,0.000045006203,0.9987256,0.0000020051928,0.000008708259,0.00012746936,0.0002442882,0.000203324,0.00025675664,0.00002333669,0.00035532762,0.00000262095],"about_ca_topic_score_codex":0.0071786353,"about_ca_topic_score_gemma":0.010217327,"teacher_disagreement_score":0.0071786353,"about_ca_system_score_codex":0.0003282064,"about_ca_system_score_gemma":0.00014033458,"threshold_uncertainty_score":0.014273703},"labels":[],"label_agreement":null},{"id":"W2011200445","doi":"10.1086/516724","title":"NGC 5548 in a Low‐Luminosity State: Implications for the Broad‐Line Region","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Jet Propulsion Laboratory; National Aeronautics and Space Administration; California Institute of Technology; Ohio State University; Science and Technology Facilities Council; CRDF Global; National Science Foundation","keywords":"Reverberation mapping; Physics; Astrophysics; Luminosity; Emission spectrum; Population; Line (geometry); Virial mass; Virial theorem; Active galactic nucleus; Astronomy; Spectral line; Galaxy; Geometry; Demography; Mathematics","score_opus":0.0231775243481639,"score_gpt":0.2736413822792298,"score_spread":0.2504638579310659,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011200445","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99936146,0.00002611608,0.00008552507,0.000012433332,8.204676e-7,0.0000011914715,0.000039824736,0.000007566663,0.00046507004],"genre_scores_gemma":[0.99979717,0.000008936921,0.000051637646,0.000006581898,0.0000016884538,0.0000015231349,0.00004580151,0.0000016154404,0.00008492704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990594,0.000011157579,0.0000043012114,0.00003430692,0.000010831719,0.00003346318],"domain_scores_gemma":[0.99946994,0.00005804735,0.00026465347,0.00007587716,0.00005357853,0.00007793222],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016008675,0.00014623246,0.00017828915,0.0004205177,0.00034281268,0.0006109073,0.00022050393,0.00020822827,0.0014765686],"category_scores_gemma":[0.00059606484,0.00008238411,0.0001549438,0.0001938169,0.00033398456,0.0002667374,0.00038425234,0.00024770334,0.0002533249],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001656338,0.000045012832,0.96032435,0.000009434951,0.000017470364,0.00027765386,0.0003883431,0.00016875686,0.033504203,0.00013546358,0.000076959535,0.0048867147],"study_design_scores_gemma":[0.0000035476673,0.000061450046,0.99746823,0.000003082693,0.000012044843,0.00028099873,0.00015437334,0.00022363488,0.0015230038,0.000057152196,0.00020956804,0.0000030139774],"about_ca_topic_score_codex":0.0046513774,"about_ca_topic_score_gemma":0.007149593,"teacher_disagreement_score":0.0046513774,"about_ca_system_score_codex":0.00026816127,"about_ca_system_score_gemma":0.000079379824,"threshold_uncertainty_score":0.009248614},"labels":[],"label_agreement":null},{"id":"W2011291483","doi":"10.1086/377602","title":"Atmospheric Models of Red Giants with Massive‐Scale Non–Local Thermodynamic Equilibrium","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Metallicity; Astrophysics; Physics; Opacity; Stars; Flux (metallurgy); Stellar atmosphere; Atmospheric models; Spectral line; Astronomy; Chemistry","score_opus":0.007151416627448633,"score_gpt":0.19839827921538528,"score_spread":0.19124686258793663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011291483","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97042835,0.00023881969,0.019183889,0.00039455923,0.000030403373,0.000024857498,0.0006795429,0.0005157561,0.008503773],"genre_scores_gemma":[0.994589,0.00014432949,0.0026821417,0.000051653333,0.00003485011,0.00002340259,0.00030788057,0.000082033825,0.0020847563],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999008,0.000030135281,0.0000054554853,0.000025082312,0.000016565278,0.000021888805],"domain_scores_gemma":[0.9996562,0.00009698391,0.0000781302,0.000027967988,0.000058895446,0.00008175358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029345087,0.00053109846,0.0005229942,0.00040342752,0.0005768077,0.0007843419,0.0014813853,0.00080245134,0.0018551993],"category_scores_gemma":[0.00088435016,0.00040863067,0.00067067286,0.00047191806,0.00050987577,0.00091191364,0.00081684586,0.00046424998,0.00035155035],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015434559,0.000058773134,0.01815378,0.000024035806,0.00007541425,0.00017708742,0.00017202181,0.9666757,0.0026572717,0.008991372,0.00058572064,0.0022745274],"study_design_scores_gemma":[0.000047458223,0.000018360683,0.0025141328,0.000002052434,0.000017340528,0.000035474437,0.00003996269,0.994561,0.00020594202,0.0019759194,0.00057108735,0.000011220267],"about_ca_topic_score_codex":0.057270348,"about_ca_topic_score_gemma":0.029249566,"teacher_disagreement_score":0.057270348,"about_ca_system_score_codex":0.0010964914,"about_ca_system_score_gemma":0.0004769244,"threshold_uncertainty_score":0.11387402},"labels":[],"label_agreement":null},{"id":"W2011415806","doi":"10.1086/383001","title":"Models for Solar Abundance Stars with Gravitational Settling and Radiative Accelerations: Application to M67 and NGC 188","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Université de Montréal","funders":"","keywords":"Astrophysics; Physics; Metallicity; Stars; Open cluster; Radiative transfer; Luminosity; Main sequence; Astronomy; Galaxy","score_opus":0.011955344949409927,"score_gpt":0.23787966521895376,"score_spread":0.22592432026954384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011415806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.948896,0.00035375994,0.04219071,0.0001305425,0.000020972448,0.000039715793,0.00037107608,0.000314733,0.007682499],"genre_scores_gemma":[0.98818773,0.00018511331,0.007894603,0.000014686863,0.000014104674,0.000035869532,0.00031326464,0.00008708682,0.0032674207],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999465,0.000011340709,0.000002993821,0.000013707177,0.00001019351,0.00001526353],"domain_scores_gemma":[0.9998223,0.00005255419,0.00003405174,0.000014316348,0.000038480168,0.00003819736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019679923,0.0005418125,0.0003682479,0.0005173282,0.00046931865,0.0005582955,0.0011961408,0.00053844246,0.0012833141],"category_scores_gemma":[0.00054785906,0.00030116312,0.00075349683,0.0004277395,0.00026063112,0.0003128263,0.0003815237,0.0003826295,0.00048641788],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009746702,0.000045935474,0.02887682,0.000053758788,0.000050430288,0.00042997926,0.0002940845,0.94857216,0.003451857,0.01003961,0.00069062784,0.0073971623],"study_design_scores_gemma":[0.000027230986,0.000035869434,0.009422314,0.000011119909,0.000023391089,0.00019994118,0.00006554277,0.985358,0.00051189796,0.0026338277,0.0016925005,0.00001838977],"about_ca_topic_score_codex":0.032865066,"about_ca_topic_score_gemma":0.017507032,"teacher_disagreement_score":0.032865066,"about_ca_system_score_codex":0.0012135544,"about_ca_system_score_gemma":0.0005757997,"threshold_uncertainty_score":0.06534755},"labels":[],"label_agreement":null},{"id":"W2011424576","doi":"10.1086/377443","title":"Oxygen Abundances in Metal‐poor Stars","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Astrophysics; Physics; Oxygen; Balmer series; Line (geometry); Observable; Forbidden mechanism; Abundance (ecology); Emission spectrum; Astronomy; Spectral line","score_opus":0.011961525739146198,"score_gpt":0.2280805918330395,"score_spread":0.2161190660938933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011424576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9168602,0.007217387,0.00025153212,0.004284729,0.0054608365,0.00008806885,0.0058039287,0.00018451356,0.059848726],"genre_scores_gemma":[0.86290556,0.0053008585,0.00048154203,0.0008834381,0.0032370405,0.00003896975,0.006993661,0.00015225094,0.12000666],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996911,0.000025431278,0.00002271182,0.000047910835,0.00017665605,0.00003612935],"domain_scores_gemma":[0.99653035,0.0002380151,0.00030057898,0.00011507013,0.0023915756,0.00042439194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055320666,0.0001682788,0.0004298515,0.0019425192,0.0006181885,0.00064958865,0.00039000466,0.0006165472,0.021259876],"category_scores_gemma":[0.0039038197,0.00010486748,0.00013065376,0.0011827878,0.00020008079,0.00047139585,0.00039111022,0.00017473483,0.0063781017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0027809094,0.00020104747,0.5035649,0.0019830337,0.00018851786,0.0020384819,0.0010278905,0.00043877555,0.04960704,0.0011972432,0.21026064,0.2267115],"study_design_scores_gemma":[0.0000987579,0.00027801926,0.8670283,0.0001733128,0.00008398044,0.00070016383,0.0005831561,0.0003593953,0.008618749,0.0007498628,0.121301375,0.000024980221],"about_ca_topic_score_codex":0.0012542598,"about_ca_topic_score_gemma":0.0022040661,"teacher_disagreement_score":0.021259876,"about_ca_system_score_codex":0.00033698138,"about_ca_system_score_gemma":0.00027277833,"threshold_uncertainty_score":0.071121335},"labels":[],"label_agreement":null},{"id":"W2011457521","doi":"10.1086/312790","title":"The Discovery of Photospheric Phosphorus and Iron in the [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Spectrum of the Hot DA White Dwarf GD 394","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Photosphere; Physics; Astrophysics; White dwarf; Ultraviolet; Far ultraviolet; Astronomy; Spectral line; Stars; Optics","score_opus":0.006516260122044916,"score_gpt":0.20387370917114433,"score_spread":0.1973574490490994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011457521","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973774,0.00012270418,0.00017626619,0.00006879569,0.00000701609,0.0000028674085,0.00014196016,0.000024613306,0.0020784182],"genre_scores_gemma":[0.9974759,0.00011513582,0.0006708174,0.000047182886,0.0000121725725,0.000003920074,0.00042414837,0.000011283252,0.001239467],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996006,0.000002453466,0.0000017763775,0.000012114819,0.000013767351,0.000009831879],"domain_scores_gemma":[0.9999614,0.0000035509595,0.0000141459395,0.0000051728375,0.000006387687,0.00000930304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006339408,0.00021919844,0.00012228229,0.0004067388,0.0003552982,0.0003203117,0.00029820713,0.00033326575,0.00094023946],"category_scores_gemma":[0.00012095882,0.00012937533,0.00010565411,0.00020884885,0.00026700864,0.00015244224,0.00035226057,0.00020431803,0.00032044583],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035802933,0.000046531768,0.05562673,0.000058176585,0.000039105318,0.0026227355,0.00021517691,0.00021668678,0.92836225,0.0006186393,0.000728996,0.0111070555],"study_design_scores_gemma":[0.00011407865,0.00040333235,0.6604949,0.000040970048,0.00015865585,0.009261598,0.00046488657,0.0016575843,0.29348993,0.0016449172,0.03222399,0.00004510175],"about_ca_topic_score_codex":0.0015780464,"about_ca_topic_score_gemma":0.002271921,"teacher_disagreement_score":0.0015780464,"about_ca_system_score_codex":0.00025962418,"about_ca_system_score_gemma":0.00008670198,"threshold_uncertainty_score":0.0031453967},"labels":[],"label_agreement":null},{"id":"W2011462635","doi":"10.1086/323525","title":"Universe Models with a Variable Cosmological “Constant” and a “Big Bounce”","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"General relativity; Spacetime; Universe; Variable (mathematics); Inflation (cosmology); Metric expansion of space; Class (philosophy); Cosmological constant; String (physics); Big Bang (financial markets)","score_opus":0.011815165519690076,"score_gpt":0.21438285286858397,"score_spread":0.20256768734889388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011462635","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7583752,0.0015558413,0.1826523,0.0018942957,0.00020278647,0.00006763808,0.000344245,0.00038018805,0.054527543],"genre_scores_gemma":[0.9642602,0.0006586474,0.023984013,0.00023180067,0.00017293416,0.000043200118,0.00026914515,0.00004673907,0.010333307],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99978954,0.00007384425,0.000011271414,0.000027151742,0.000041649604,0.000056602097],"domain_scores_gemma":[0.9994892,0.000096396965,0.00013571366,0.000079122205,0.00006145259,0.00013809965],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004445045,0.0010475836,0.00080825534,0.0008386916,0.0009862634,0.0013763898,0.0012575268,0.0015267746,0.0021923939],"category_scores_gemma":[0.0016834129,0.00041859492,0.0008550965,0.000616891,0.0017630408,0.001989631,0.0021934405,0.00094798027,0.00027035514],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000069379814,0.000049255024,0.0011647651,0.000072128176,0.000068399095,0.00044713626,0.0002962534,0.08066169,0.0011576102,0.9110818,0.0012294354,0.0037021118],"study_design_scores_gemma":[0.00015640206,0.000067311834,0.0011064769,0.000026354868,0.00006057144,0.00044306286,0.00022375076,0.43507588,0.00057336106,0.559225,0.002984552,0.00005723593],"about_ca_topic_score_codex":0.0040687886,"about_ca_topic_score_gemma":0.0041325805,"teacher_disagreement_score":0.0040687886,"about_ca_system_score_codex":0.00067962,"about_ca_system_score_gemma":0.0005298475,"threshold_uncertainty_score":0.008090198},"labels":[],"label_agreement":null},{"id":"W2011490256","doi":"10.1086/523619","title":"The Milky Way Tomography with SDSS. I. Stellar Number Density Distribution","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1326,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Physics; Astrophysics; Milky Way; Halo; Sky; Galaxy; Thick disk; Star count; Dwarf galaxy; Surface brightness; Stars; Astronomy","score_opus":0.007996869845049092,"score_gpt":0.20119975718322067,"score_spread":0.19320288733817156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011490256","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03748835,0.0011241188,0.043357696,0.0006470967,0.0002285166,0.00030124173,0.73739594,0.13366072,0.04579632],"genre_scores_gemma":[0.12406951,0.00088333647,0.09231007,0.00052972045,0.00018763998,0.00080120104,0.7585588,0.00915335,0.013506414],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99943227,0.00008550389,0.00006468419,0.00015198502,0.00019479972,0.00007072666],"domain_scores_gemma":[0.9987367,0.00008961038,0.00028552007,0.00039535013,0.00036090432,0.00013202269],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011276589,0.00091673195,0.00062157377,0.0054645278,0.00042821743,0.0015357272,0.00091237074,0.00043674096,0.015415429],"category_scores_gemma":[0.0031130114,0.00043219846,0.00063829654,0.0071021323,0.00024400889,0.0012414993,0.0017042957,0.0008293809,0.02147784],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002760673,0.00016282644,0.053428754,0.00048156772,0.00028025964,0.00032070014,0.00050321186,0.0044476846,0.0045787147,0.011126976,0.7946161,0.12977709],"study_design_scores_gemma":[0.00017999925,0.00005056175,0.097273186,0.00014268147,0.00008391908,0.0003261954,0.00029329,0.020860873,0.005435979,0.015798442,0.85946715,0.00008774671],"about_ca_topic_score_codex":0.010514323,"about_ca_topic_score_gemma":0.0072880974,"teacher_disagreement_score":0.015415429,"about_ca_system_score_codex":0.0006617236,"about_ca_system_score_gemma":0.00093018933,"threshold_uncertainty_score":0.05156976},"labels":[],"label_agreement":null},{"id":"W2011506636","doi":"10.1086/341178","title":"Discovery of Radio Pulsations from the X-Ray Pulsar J0205+6449 in Supernova Remnant 3C 58 with the Green Bank Telescope","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Supernova remnant; Radio telescope; X-ray pulsar; Luminosity; Green Bank Telescope; Astronomy; Telescope; Radio spectrum; Spectral index; Binary pulsar; Pulsar planet; Supernova; Millisecond pulsar; Spectral line; Galaxy","score_opus":0.010538694055908111,"score_gpt":0.20004700685353458,"score_spread":0.18950831279762648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011506636","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993901,0.00010116267,0.000109535955,0.0000152263465,0.0000048911347,0.0000032416167,0.000046740017,0.000006449061,0.00032262577],"genre_scores_gemma":[0.9988111,0.00014254286,0.0004471206,0.00003220134,0.000015014597,0.0000056041326,0.00022440394,0.000003608273,0.00031844567],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991155,0.000008622911,0.00000673734,0.000018868002,0.00002995883,0.000024218494],"domain_scores_gemma":[0.9997696,0.000021915614,0.0000822155,0.000032940865,0.000025574953,0.00006772156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021864842,0.00020459291,0.00020342832,0.00054183806,0.00047015815,0.0005173514,0.000277622,0.0002891912,0.00075314357],"category_scores_gemma":[0.00046508422,0.00019931553,0.00014154827,0.00033913218,0.0003249429,0.00019300953,0.00065983285,0.00024283546,0.00037872148],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045587015,0.00015823264,0.7623909,0.00005505778,0.0001226436,0.01043064,0.0008707333,0.0003990153,0.20399322,0.00071926805,0.0008328531,0.019571489],"study_design_scores_gemma":[0.000053966818,0.0003575362,0.9751891,0.000019177607,0.000060413284,0.007112352,0.00020894299,0.0006606043,0.011781746,0.00018794049,0.0043487367,0.000019492321],"about_ca_topic_score_codex":0.0021298302,"about_ca_topic_score_gemma":0.0036870835,"teacher_disagreement_score":0.0021298302,"about_ca_system_score_codex":0.00021900832,"about_ca_system_score_gemma":0.0001695887,"threshold_uncertainty_score":0.00423491},"labels":[],"label_agreement":null},{"id":"W2011516147","doi":"10.1088/0004-637x/704/2/1710","title":"ASTEROSEISMIC ANALYSIS OF THE PRE-MAIN-SEQUENCE STARS IN NGC 2264","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université du Québec à Montréal; University of British Columbia; Université de Montréal; Saint Mary's University","funders":"","keywords":"Physics; Stars; Astrophysics; Photometry (optics); Spectral line; Astronomy; Oscillation (cell signaling); Open cluster; K-type main-sequence star; T Tauri star","score_opus":0.011712692661935552,"score_gpt":0.24063761642374282,"score_spread":0.22892492376180726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011516147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993362,0.000019004701,0.0001155787,0.0000042304114,7.352868e-7,0.0000010838556,0.00014148472,0.000011834446,0.00036994394],"genre_scores_gemma":[0.9989753,0.00001644797,0.00021201068,0.0000019089068,9.782024e-7,0.0000010554187,0.0005045682,0.0000025979286,0.0002852483],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999962,0.000004717293,0.0000027765382,0.000011775447,0.000010500873,0.000008277472],"domain_scores_gemma":[0.99986804,0.000016149534,0.000039536357,0.000018691991,0.00001913088,0.000038324193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007270318,0.00015241637,0.0001134368,0.00082823186,0.0002454839,0.00021454542,0.00013240523,0.00013905251,0.0009686633],"category_scores_gemma":[0.00027742196,0.000061218016,0.00016385796,0.00044633984,0.00015258505,0.000093557195,0.00018381348,0.00007492292,0.00020785259],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024469796,0.00005190228,0.86960524,0.000033421173,0.000048584778,0.0004680324,0.0002917374,0.0035890548,0.11202281,0.0003842711,0.00024358506,0.01301665],"study_design_scores_gemma":[0.0000023828368,0.0000260367,0.99534094,0.0000012134482,0.00000836277,0.00012308013,0.00006338596,0.0021515545,0.0018085992,0.00006664461,0.00040513618,0.0000027302847],"about_ca_topic_score_codex":0.006894374,"about_ca_topic_score_gemma":0.0074671498,"teacher_disagreement_score":0.006894374,"about_ca_system_score_codex":0.00029638858,"about_ca_system_score_gemma":0.000113617476,"threshold_uncertainty_score":0.013708472},"labels":[],"label_agreement":null},{"id":"W2011570622","doi":"10.1088/0004-637x/745/1/65","title":"UNVEILING THE PHYSICAL PROPERTIES AND KINEMATICS OF MOLECULAR GAS IN THE ANTENNAE GALAXIES (NGC 4038/9) THROUGH HIGH-RESOLUTION CO (<i>J</i>= 3-2) OBSERVATIONS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Physics; Galaxy; Star formation; Line (geometry); Surface brightness; Resolution (logic); Wavelength; Astronomy; Geometry; Optics","score_opus":0.034925059740030545,"score_gpt":0.22342797641430434,"score_spread":0.1885029166742738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011570622","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993777,0.000047807236,0.000058457965,0.000010485974,4.833738e-7,0.0000016215573,0.00008641504,0.000010394988,0.00040665054],"genre_scores_gemma":[0.9992601,0.000038330196,0.0003311375,0.000007303769,0.0000035398505,0.0000031733796,0.00019856895,0.000003568495,0.0001541759],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990106,0.000006352445,0.0000033543417,0.000037868802,0.000020572266,0.000030704727],"domain_scores_gemma":[0.999866,0.0000080447935,0.000048856225,0.000012256787,0.000011330477,0.000053482887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000088631765,0.00022903344,0.00021669027,0.0008071705,0.0002929396,0.00035320566,0.00024082972,0.00022005974,0.0008037469],"category_scores_gemma":[0.00019335913,0.00023833597,0.00014138318,0.0004758216,0.00020855771,0.0003163947,0.00064328423,0.00018335014,0.00022769764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000120563185,0.000053744752,0.7595869,0.000039918916,0.00007591754,0.00056198967,0.0008983414,0.00085366797,0.22640988,0.00025772263,0.0003460991,0.010795215],"study_design_scores_gemma":[0.000004171048,0.0000243548,0.99705017,0.000002792988,0.000009957267,0.0001823519,0.00013697035,0.00057277444,0.0013205523,0.00005341111,0.00063846837,0.0000040108102],"about_ca_topic_score_codex":0.0069862115,"about_ca_topic_score_gemma":0.018694017,"teacher_disagreement_score":0.0069862115,"about_ca_system_score_codex":0.00033684843,"about_ca_system_score_gemma":0.00010967642,"threshold_uncertainty_score":0.013891101},"labels":[],"label_agreement":null},{"id":"W2011606526","doi":"10.1086/505781","title":"A Search for Kilogauss Magnetic Fields in White Dwarfs and Hot Subdwarf Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Royal Military College of Canada","funders":"","keywords":"White dwarf; Subdwarf; Physics; Astrophysics; Stars; Magnetic field; Polarization (electrochemistry); Astronomy","score_opus":0.010681033713891596,"score_gpt":0.23032027941685018,"score_spread":0.2196392457029586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011606526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987801,0.00013569965,0.000043164866,0.00008042178,0.0000038002777,0.0000034454472,0.000099392055,0.0000027907242,0.0008511638],"genre_scores_gemma":[0.99932706,0.0000516774,0.000052381733,0.000033821478,0.000011004285,0.0000020017696,0.00012101153,0.0000012709165,0.00039980773],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986315,0.00002695384,0.0000103434595,0.00003723303,0.000026435026,0.000035787332],"domain_scores_gemma":[0.9988827,0.00023306231,0.0003543785,0.00005165181,0.00015808031,0.00032005782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030519234,0.00011148711,0.00015872534,0.0017251018,0.00068373495,0.0006319456,0.00027020773,0.00041800298,0.0023690003],"category_scores_gemma":[0.0012449761,0.000092531984,0.00011350268,0.0008780433,0.00045163123,0.0003436851,0.0004672474,0.00023878472,0.00024241813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000236078,0.00005084011,0.9905811,0.00001546398,0.000018867957,0.00015643287,0.00037600417,0.00001994443,0.002612986,0.000125627,0.00016598351,0.005640646],"study_design_scores_gemma":[0.000006497793,0.000049106813,0.9980469,0.000003945924,0.000010351014,0.00027924706,0.00096041785,0.000037288908,0.0001440582,0.00011356018,0.00034687764,0.0000017545705],"about_ca_topic_score_codex":0.007941112,"about_ca_topic_score_gemma":0.011888896,"teacher_disagreement_score":0.007941112,"about_ca_system_score_codex":0.0003349367,"about_ca_system_score_gemma":0.0004138306,"threshold_uncertainty_score":0.015789807},"labels":[],"label_agreement":null},{"id":"W2011696329","doi":"10.1088/0004-637x/726/2/78","title":"PHASE TRANSITION GENERATED COSMOLOGICAL MAGNETIC FIELD AT LARGE SCALES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Laurentian University","funders":"","keywords":"Amplitude; Magnetic field; Big Bang nucleosynthesis; Cosmology; Nucleosynthesis; Gravitational wave; Gravitation; Spectral density; Phase (matter); Field (mathematics)","score_opus":0.010856681528515107,"score_gpt":0.3174178034122649,"score_spread":0.3065611218837498,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011696329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9881825,0.00016282214,0.007275925,0.000109478446,0.0000131786655,0.000007646673,0.00015493613,0.000119659155,0.0039738254],"genre_scores_gemma":[0.99907374,0.00002694227,0.0006968617,0.000012723569,0.00000896457,0.0000033236263,0.00008226483,0.000008835626,0.00008633111],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999565,0.000009816273,0.0000011647182,0.000014479493,0.0000073903466,0.000010685136],"domain_scores_gemma":[0.9997328,0.000075825774,0.000101135316,0.000032588538,0.0000145139375,0.000043100106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017260136,0.00020132544,0.00016610624,0.00027533452,0.00019491272,0.00041327556,0.00020150191,0.00018895738,0.00072580937],"category_scores_gemma":[0.0011790134,0.00016534458,0.00014505436,0.00018849869,0.00028973955,0.0003809529,0.00037842212,0.0003726242,0.000111043],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011593156,0.00023145681,0.31132635,0.00031320332,0.0004534828,0.0017332638,0.0008569446,0.12605017,0.26082957,0.23646368,0.004023975,0.05655855],"study_design_scores_gemma":[0.00029774,0.0003196911,0.49651417,0.00003794274,0.0001544892,0.00085214106,0.00017395383,0.3203613,0.03947124,0.13053216,0.011188078,0.00009707303],"about_ca_topic_score_codex":0.0008053155,"about_ca_topic_score_gemma":0.0008772677,"teacher_disagreement_score":0.0008053155,"about_ca_system_score_codex":0.0002768301,"about_ca_system_score_gemma":0.00013148112,"threshold_uncertainty_score":0.0024280548},"labels":[],"label_agreement":null},{"id":"W2011811871","doi":"10.1086/432642","title":"CO in H<scp>i</scp>Self‐absorbed Clouds in Perseus","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Calgary","funders":"","keywords":"Radiative transfer; Molecular cloud; Extinction (optical mineralogy); Stars; Monte Carlo method; Galaxy","score_opus":0.008943228383481475,"score_gpt":0.24517823625691415,"score_spread":0.23623500787343268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011811871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996314,0.00003537404,0.000052583553,0.000007898414,0.0000010223769,0.0000013517285,0.00004427452,0.0000066733946,0.00021936576],"genre_scores_gemma":[0.9997497,0.000014941162,0.00008053924,0.000006971496,0.0000016142086,0.0000011146577,0.00006436488,0.0000019637773,0.00007869388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999206,0.0000055606492,0.0000029347532,0.00002822824,0.000021321513,0.000021281374],"domain_scores_gemma":[0.9998301,0.000028358543,0.000055116736,0.000017416758,0.00002843727,0.000040575702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010575753,0.00024169737,0.00020465926,0.0007479189,0.00042899922,0.0003826532,0.00026164317,0.00020623833,0.00038655248],"category_scores_gemma":[0.00022454993,0.00019274415,0.00010507549,0.0005875463,0.0004290753,0.00026225933,0.00043106038,0.00013637193,0.000105557934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023472568,0.00004957803,0.9398377,0.000030370733,0.00008677267,0.0010992929,0.00086760713,0.0025872388,0.045828354,0.00025197235,0.00023390334,0.008892409],"study_design_scores_gemma":[0.000016701202,0.000048074406,0.9931958,0.0000056658314,0.00001543902,0.00020933634,0.00029313244,0.0025006274,0.0031286222,0.00012689628,0.00045337944,0.0000063319626],"about_ca_topic_score_codex":0.035723194,"about_ca_topic_score_gemma":0.05313358,"teacher_disagreement_score":0.035723194,"about_ca_system_score_codex":0.00062387186,"about_ca_system_score_gemma":0.0002278905,"threshold_uncertainty_score":0.07103056},"labels":[],"label_agreement":null},{"id":"W2011815073","doi":"10.1088/0004-637x/778/2/106","title":"BROADBAND PULSATIONS FROM PSR B1821–24: IMPLICATIONS FOR EMISSION MODELS AND THE PULSAR POPULATION OF M28","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Université Laval","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Millisecond pulsar; Globular cluster; Population; Neutron star; Pulsar planet; Cluster (spacecraft); Telescope","score_opus":0.020886193585565673,"score_gpt":0.3187603068090999,"score_spread":0.29787411322353424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011815073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99925286,0.000038559134,0.00027823594,0.000034941615,9.356694e-7,0.0000032485175,0.00010042529,0.000014160041,0.00027661544],"genre_scores_gemma":[0.9989662,0.00003797296,0.00040474255,0.000015022329,0.000006817136,0.000006843844,0.00040034662,0.000012177083,0.00014983077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998926,0.0000131603,0.0000063725965,0.000043537082,0.000022318447,0.000022035572],"domain_scores_gemma":[0.9994925,0.00008147728,0.0002046878,0.0000677765,0.00004419817,0.00010930475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030670472,0.00046432303,0.0004458506,0.00069461256,0.00044608206,0.00056614354,0.00092025875,0.00038858198,0.0013984125],"category_scores_gemma":[0.0008798531,0.00021257396,0.00035281008,0.0005077963,0.00034917952,0.00034624006,0.0006554789,0.00032357126,0.0004818837],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031321196,0.00009569019,0.9452778,0.00004284292,0.000077952725,0.0003334116,0.00042957085,0.00880658,0.035338964,0.00070813857,0.00036761299,0.008208244],"study_design_scores_gemma":[0.000060718263,0.00015459667,0.9638904,0.000012563485,0.000044034932,0.00030737423,0.0002343939,0.030356864,0.0023257218,0.0013798198,0.0012149845,0.000018535588],"about_ca_topic_score_codex":0.003879067,"about_ca_topic_score_gemma":0.0038135282,"teacher_disagreement_score":0.003879067,"about_ca_system_score_codex":0.000755189,"about_ca_system_score_gemma":0.0002217151,"threshold_uncertainty_score":0.0077129602},"labels":[],"label_agreement":null},{"id":"W2011819599","doi":"10.1088/0004-637x/787/2/107","title":"THE SPATIAL STRUCTURE OF YOUNG STELLAR CLUSTERS. I. SUBCLUSTERS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Stars; Physics; Halo; RADIUS; Cluster (spacecraft); Astronomy; Galaxy","score_opus":0.004747522827681668,"score_gpt":0.20934360638041746,"score_spread":0.20459608355273579,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011819599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99653935,0.00042712924,0.00072683045,0.00002305173,0.0000014840829,0.000010912006,0.0005904071,0.000032362084,0.0016485912],"genre_scores_gemma":[0.9972728,0.00017091163,0.0009731777,0.0000061790365,0.000003713202,0.0000071150803,0.00091518287,0.000008880043,0.00064205966],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997582,0.000022892928,0.000025652853,0.00008853463,0.00006200793,0.000042782674],"domain_scores_gemma":[0.9986212,0.00020633284,0.0005677924,0.0001219731,0.00027765942,0.00020502842],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002470034,0.00011574064,0.0001700249,0.0024523467,0.00045975865,0.00071668986,0.00021846025,0.0000989439,0.001934204],"category_scores_gemma":[0.0014931643,0.00012409549,0.00014940112,0.0018507772,0.00046067795,0.00037004228,0.0010719064,0.00010919618,0.00061493745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009989185,0.000008239214,0.9744285,0.00004392905,0.00002190477,0.00007299843,0.0010947745,0.00076313555,0.0050470396,0.0012325313,0.00032452706,0.016862571],"study_design_scores_gemma":[0.0000035135802,0.000024758509,0.9957339,0.000010406692,0.000009728024,0.00020553898,0.00040224413,0.0009679183,0.00055873237,0.0006077216,0.001470674,0.000004731873],"about_ca_topic_score_codex":0.0077025583,"about_ca_topic_score_gemma":0.009915673,"teacher_disagreement_score":0.0077025583,"about_ca_system_score_codex":0.0004679494,"about_ca_system_score_gemma":0.00037296998,"threshold_uncertainty_score":0.015315473},"labels":[],"label_agreement":null},{"id":"W2011829982","doi":"10.1086/509909","title":"Cosmological Constraints from the Red‐Sequence Cluster Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Canadian Institute for Theoretical Astrophysics; York University; University of Toronto","funders":"","keywords":"Cluster (spacecraft); Calibration; Consistency (knowledge bases); Relation (database); Sky; Sample (material); Cosmology","score_opus":0.02345193767063658,"score_gpt":0.2488519423178335,"score_spread":0.22540000464719692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011829982","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7939106,0.0034610194,0.03092845,0.0015828182,0.00009064071,0.00013632058,0.10893476,0.001138868,0.059816454],"genre_scores_gemma":[0.86876696,0.0014890272,0.021762785,0.00050711364,0.00015137567,0.00008290036,0.09942595,0.0005680349,0.00724574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99950755,0.00013038855,0.000023729606,0.00011793664,0.0001679879,0.00005243608],"domain_scores_gemma":[0.9979971,0.0005830402,0.00040139613,0.0004207149,0.00038143285,0.0002163254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012004268,0.0005178309,0.00047232237,0.0012977355,0.0005909641,0.0010134378,0.00063597265,0.00026461552,0.009486224],"category_scores_gemma":[0.0037526335,0.0002917631,0.0004425953,0.0023182794,0.00020979406,0.0003870953,0.0007253426,0.00071190234,0.0015457253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046214947,0.00014446345,0.56494,0.0006089573,0.0009645038,0.0007065531,0.0017219583,0.06371081,0.010923482,0.1143879,0.13828528,0.10314396],"study_design_scores_gemma":[0.000026708114,0.000032147418,0.90055186,0.00014917388,0.000081452155,0.00021306839,0.00017847732,0.016819447,0.001109325,0.009813263,0.0709556,0.00006938513],"about_ca_topic_score_codex":0.08392136,"about_ca_topic_score_gemma":0.09629359,"teacher_disagreement_score":0.08392136,"about_ca_system_score_codex":0.001080887,"about_ca_system_score_gemma":0.0011592568,"threshold_uncertainty_score":0.16686577},"labels":[],"label_agreement":null},{"id":"W2011858560","doi":"10.1086/377495","title":"Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Equipartition theorem; Magnetohydrodynamics; Molecular cloud; Shock wave; Mechanics; Amplitude; Classical mechanics; Kinetic energy; Computational physics; Magnetic field; Astrophysics; Stars; Quantum mechanics","score_opus":0.009655304840509459,"score_gpt":0.22808089584309324,"score_spread":0.21842559100258377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2011858560","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975879,0.000027618837,0.00076124247,0.00009657212,0.000010705631,0.000013740561,0.000076630226,0.000019738574,0.0014057739],"genre_scores_gemma":[0.99907565,0.00002417433,0.0005227507,0.000026608506,0.0000057755224,0.000009876728,0.00007991559,0.0000075365742,0.0002477083],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998388,0.000029529703,0.0000075504286,0.000017644732,0.000024804922,0.00008167584],"domain_scores_gemma":[0.9993913,0.0001885487,0.00010908917,0.000041856158,0.00007301932,0.00019614957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033608387,0.0005108989,0.00063839206,0.0004674539,0.0010780827,0.0012642195,0.0010243967,0.0011137001,0.0011171417],"category_scores_gemma":[0.0014379922,0.0003161224,0.0006478791,0.00044431427,0.001266436,0.0006649579,0.0011282241,0.00080465496,0.00011041032],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004137916,0.00022362312,0.01625652,0.00003713871,0.000080780184,0.0004768029,0.00016906059,0.9719525,0.0059897783,0.0032068326,0.0001952331,0.000998045],"study_design_scores_gemma":[0.000058080725,0.000059554604,0.0020474473,0.0000037801617,0.000011360268,0.000012761685,0.000052832394,0.996851,0.0006037439,0.00021981004,0.000072900075,0.0000067979413],"about_ca_topic_score_codex":0.051455144,"about_ca_topic_score_gemma":0.018116783,"teacher_disagreement_score":0.051455144,"about_ca_system_score_codex":0.0015760214,"about_ca_system_score_gemma":0.001259708,"threshold_uncertainty_score":0.10231125},"labels":[],"label_agreement":null},{"id":"W2012003645","doi":"10.1086/511676","title":"<i>Spitzer</i> Identifications and Classifications of Submillimeter Galaxies in Giant, High-Redshift, Lyα-Emission-Line Nebulae","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Spitzer Space Telescope; Astronomy; Galaxy; Redshift; Infrared; Star formation; Active galactic nucleus; Starlight; Luminous infrared galaxy; Population; Telescope; Stars","score_opus":0.011404104565937176,"score_gpt":0.23421477010349714,"score_spread":0.22281066553755996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012003645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979122,0.000081171,0.00023165449,0.000035460984,0.0000034203576,0.000011139729,0.0004496235,0.000049329985,0.0012259377],"genre_scores_gemma":[0.99776506,0.000034484037,0.000837899,0.000033439173,0.00001202891,0.000010410948,0.0010460531,0.000006588948,0.00025410583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998858,0.000009465656,0.000014545314,0.000027474469,0.000024940015,0.00003776828],"domain_scores_gemma":[0.99883634,0.0000944365,0.000615207,0.00009184579,0.00015507026,0.00020715204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032901496,0.00018731867,0.00013488469,0.0041031,0.00023182586,0.0005907912,0.0003441825,0.0002186997,0.0020624362],"category_scores_gemma":[0.0006574547,0.000097652155,0.00020945728,0.0007931549,0.00031209676,0.0003467471,0.00047424246,0.00016241954,0.000474576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005936464,0.000018064145,0.9851246,0.000007277522,0.00001595553,0.00006115866,0.00017948037,0.0000771605,0.009947237,0.00010091613,0.00031144,0.0040973444],"study_design_scores_gemma":[0.0000021126393,0.000012185164,0.9992137,0.0000012136195,0.0000028837417,0.00008930187,0.00006330814,0.00012019115,0.0003515228,0.000024225306,0.000118132804,0.000001201892],"about_ca_topic_score_codex":0.0035984665,"about_ca_topic_score_gemma":0.007838378,"teacher_disagreement_score":0.0041031,"about_ca_system_score_codex":0.00026376944,"about_ca_system_score_gemma":0.000116377865,"threshold_uncertainty_score":0.007155001},"labels":[],"label_agreement":null},{"id":"W2012008182","doi":"10.1086/525851","title":"16-20 μm Spectra of Carbon Nanoparticles","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Spectral line; Carbon fibers; Astrophysics; Carbon Nanoparticles; Interstellar medium; Astrochemistry; Emission spectrum; Line (geometry); Nanoparticle; Astronomy; Galaxy; Materials science","score_opus":0.009134362042387456,"score_gpt":0.2356569463006935,"score_spread":0.22652258425830604,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012008182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94500214,0.0027788333,0.01051757,0.0006235687,0.00020693483,0.000036082656,0.0008904482,0.00057549425,0.039368972],"genre_scores_gemma":[0.9829245,0.00070112676,0.0055461023,0.0003901789,0.00004643103,0.000077836434,0.0006616254,0.00009405015,0.009558089],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998895,0.0000074897494,0.000002984739,0.000034592507,0.000043287135,0.0000221365],"domain_scores_gemma":[0.9997559,0.00008281376,0.00004870158,0.000018987641,0.00006299201,0.00003052871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001295379,0.00028182685,0.0001240898,0.000448403,0.00025383238,0.00017391205,0.00026318812,0.00042314295,0.007403988],"category_scores_gemma":[0.00019827606,0.00008255304,0.00016139046,0.00031346548,0.00023633784,0.00020871108,0.00019865358,0.0006398899,0.0005501324],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012273053,0.000056363537,0.0006398409,0.00013056761,0.000019216253,0.00019432417,0.00006956059,0.0003943989,0.9899991,0.00044963873,0.0013821776,0.006542049],"study_design_scores_gemma":[0.000018229704,0.00020640116,0.021487117,0.000031199383,0.000023414728,0.00045498484,0.00013400866,0.0028654968,0.96716344,0.00034821447,0.0072506364,0.000016863194],"about_ca_topic_score_codex":0.0008154771,"about_ca_topic_score_gemma":0.0010024962,"teacher_disagreement_score":0.007403988,"about_ca_system_score_codex":0.000461921,"about_ca_system_score_gemma":0.00009355059,"threshold_uncertainty_score":0.02476883},"labels":[],"label_agreement":null},{"id":"W2012299678","doi":"10.1088/0004-637x/760/1/72","title":"COSMIC EVOLUTION OF STAR FORMATION ENHANCEMENT IN CLOSE MAJOR-MERGER GALAXY PAIRS SINCE<i>z</i>= 1","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Star formation; Luminosity; Redshift; Galaxy formation and evolution; Halo; Cosmic infrared background; Luminous infrared galaxy","score_opus":0.00708478967077183,"score_gpt":0.21216968608405545,"score_spread":0.20508489641328362,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012299678","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952054,0.00006202417,0.000027343274,0.000007942547,6.8349283e-7,0.0000011279052,0.000105719395,0.000005520647,0.0002690338],"genre_scores_gemma":[0.9996933,0.00002263923,0.00002676227,0.0000035985809,0.0000026875816,0.0000010289773,0.00018308779,0.0000011572192,0.00006568789],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998745,0.0000177386,0.000008509108,0.000039139955,0.000021407366,0.000038732247],"domain_scores_gemma":[0.9990746,0.000088755005,0.0004522352,0.000049036535,0.00006282003,0.0002726338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000204252,0.0001685248,0.00018139025,0.0011674872,0.00021241208,0.00054085354,0.00015634345,0.00024471415,0.0010953523],"category_scores_gemma":[0.00086090807,0.00010596092,0.00017710972,0.00073943834,0.00023964206,0.0002347982,0.00041832487,0.00019570584,0.00019635967],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001338243,0.000022715627,0.9891944,0.0000081838125,0.000035597408,0.00012776583,0.00016862326,0.00017507694,0.0069405427,0.00011983768,0.0000654942,0.0030079947],"study_design_scores_gemma":[6.881962e-7,0.000021020971,0.99955004,3.530325e-7,0.000004019348,0.00006718959,0.000022408825,0.000081404156,0.00018795849,0.000008679499,0.00005544244,8.14679e-7],"about_ca_topic_score_codex":0.0025174625,"about_ca_topic_score_gemma":0.0032971576,"teacher_disagreement_score":0.0025174625,"about_ca_system_score_codex":0.00041122548,"about_ca_system_score_gemma":0.0000985472,"threshold_uncertainty_score":0.005005598},"labels":[],"label_agreement":null},{"id":"W2012392189","doi":"10.1086/503537","title":"The Radius‐Luminosity Relationship for Active Galactic Nuclei: The Effect of Host‐Galaxy Starlight on Luminosity Measurements","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":408,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Starlight; Active galactic nucleus; Luminosity; Stars; Ultraviolet astronomy; Background radiation","score_opus":0.0129810324377488,"score_gpt":0.22700946046414192,"score_spread":0.2140284280263931,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012392189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97848994,0.0017625745,0.016581962,0.00008998122,0.000010930941,0.0000131058505,0.00034851365,0.00030200373,0.0024010458],"genre_scores_gemma":[0.996029,0.00015802876,0.0031112875,0.000023571842,0.000009720678,0.0000047511394,0.00031244222,0.000060817998,0.00029033248],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986504,0.00051207084,0.0000827989,0.00037555982,0.00029533994,0.00008380855],"domain_scores_gemma":[0.9878781,0.005626462,0.0028494792,0.0019741096,0.0013540351,0.0003179483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019579458,0.00037274268,0.00033564886,0.0007471791,0.00019441158,0.0005718733,0.00062345574,0.00041652028,0.0008487061],"category_scores_gemma":[0.012157783,0.00028343982,0.00030227232,0.0005450002,0.00037967745,0.00082943507,0.00050014345,0.0004453659,0.0007012195],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014750558,0.000025487298,0.9046553,0.00007920329,0.00016059,0.00019882766,0.00038850002,0.004330932,0.060106963,0.00034699833,0.0002776213,0.029282246],"study_design_scores_gemma":[0.000005310546,0.00015688455,0.9548539,0.000014040426,0.00007061549,0.00081383146,0.0000660228,0.010393302,0.032015074,0.0002266051,0.0013572638,0.00002712813],"about_ca_topic_score_codex":0.0028425679,"about_ca_topic_score_gemma":0.00444023,"teacher_disagreement_score":0.0028425679,"about_ca_system_score_codex":0.00038572148,"about_ca_system_score_gemma":0.00013419974,"threshold_uncertainty_score":0.010354757},"labels":[],"label_agreement":null},{"id":"W2012447694","doi":"10.1088/0004-637x/766/2/85","title":"<i>HERSCHEL</i>OBSERVATIONS OF THE W3 GMC: CLUES TO THE FORMATION OF CLUSTERS OF HIGH-MASS STARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Canadian Institute for Theoretical Astrophysics; National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Star formation; Stars; Physics; Astrophysics; Cluster (spacecraft); Star cluster; High mass; Astronomy; Computer science","score_opus":0.013842951464382925,"score_gpt":0.22272145738824442,"score_spread":0.2088785059238615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012447694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96525204,0.0011138492,0.005040169,0.0008430091,0.00004306203,0.000043327113,0.0128263,0.0005975923,0.014240726],"genre_scores_gemma":[0.97194266,0.00036177572,0.012775669,0.00031752395,0.00008939773,0.000029277282,0.011223274,0.00014639729,0.0031139941],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994004,0.000004905372,0.000002589482,0.000013065818,0.000019772477,0.000019549],"domain_scores_gemma":[0.99974173,0.000027042426,0.00008447105,0.000050277737,0.0000380759,0.000058447193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024371082,0.00017119422,0.000102048674,0.00084840006,0.00040666416,0.00047071354,0.000280409,0.00034708396,0.00337842],"category_scores_gemma":[0.0002781333,0.00011127321,0.00018587433,0.0011530635,0.00023762621,0.00036060723,0.0005118806,0.0003649587,0.0008894755],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000432622,0.00012972426,0.6745222,0.000283724,0.00022497926,0.0009594177,0.0008618725,0.0020740426,0.23600268,0.0027988346,0.021276794,0.06043305],"study_design_scores_gemma":[0.000017227389,0.000027994563,0.96918184,0.0000258649,0.00002648822,0.00020580756,0.00012101504,0.0011602014,0.011897344,0.0005572074,0.016761392,0.00001759965],"about_ca_topic_score_codex":0.011391076,"about_ca_topic_score_gemma":0.028221196,"teacher_disagreement_score":0.011391076,"about_ca_system_score_codex":0.00032158673,"about_ca_system_score_gemma":0.00021664567,"threshold_uncertainty_score":0.022649527},"labels":[],"label_agreement":null},{"id":"W2012487415","doi":"10.1088/0004-637x/720/2/1727","title":"THE HIGH-ORDER MULTIPLICITY OF UNUSUALLY WIDE M DWARF BINARIES: ELEVEN NEW TRIPLE AND QUADRUPLE SYSTEMS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Multiplicity (mathematics); Binary number; Stars; Stellar classification; Brown dwarf; Low Mass; Binary star; Range (aeronautics); Fraction (chemistry)","score_opus":0.008042440979332287,"score_gpt":0.21927277828978248,"score_spread":0.21123033731045018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012487415","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995819,0.00008264677,0.00010611731,0.000005798294,0.0000012041879,0.000001473314,0.00006345662,0.0000054534853,0.0001521029],"genre_scores_gemma":[0.9992225,0.000049312956,0.00025215762,0.000009961276,0.0000047588687,0.0000016545415,0.0003196444,0.0000024755245,0.00013753242],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995745,0.000027788828,0.000033092107,0.00014641526,0.00013246642,0.00008563603],"domain_scores_gemma":[0.99911803,0.00014437134,0.0003165267,0.00009993903,0.00006259813,0.00025845962],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026294182,0.00019575289,0.0004229441,0.0013614965,0.00068617245,0.0007851607,0.0003302733,0.00028416145,0.0009876488],"category_scores_gemma":[0.0008495435,0.00019086794,0.0001780452,0.00078661507,0.000367571,0.00040573813,0.0010750935,0.0002819722,0.00028620963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009622165,0.00003188952,0.97881055,0.000020323756,0.00002633101,0.00034774176,0.00030222975,0.000103604456,0.01104688,0.000110709356,0.00010721092,0.00899639],"study_design_scores_gemma":[0.000003342803,0.00004706321,0.9957983,0.0000033759293,0.000011581589,0.0014728055,0.00017428567,0.00029581808,0.0014722102,0.00010037939,0.0006150297,0.0000057342977],"about_ca_topic_score_codex":0.0011370232,"about_ca_topic_score_gemma":0.0023008708,"teacher_disagreement_score":0.0013614965,"about_ca_system_score_codex":0.00025160986,"about_ca_system_score_gemma":0.00015931412,"threshold_uncertainty_score":0.0033040047},"labels":[],"label_agreement":null},{"id":"W2012511602","doi":"10.1086/422908","title":"Orbital Roulette: A New Method of Gravity Estimation from Observed Motions","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Randomness; Virial theorem; Estimator; A priori and a posteriori; Test particle; Moment (physics); Orbital elements; Gravitational potential; Celestial mechanics","score_opus":0.028905936638869825,"score_gpt":0.34952178251275384,"score_spread":0.32061584587388403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012511602","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0061034104,0.000111365836,0.9922321,0.000038949333,0.00003262206,0.000029328137,0.00008056432,0.0009776321,0.000393975],"genre_scores_gemma":[0.155467,0.00021087338,0.8409527,0.00008087053,0.00016444399,0.00017345573,0.0007129735,0.00040406102,0.0018336028],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99826884,0.0006534714,0.00008111131,0.00037487558,0.00051791494,0.00010373899],"domain_scores_gemma":[0.9956285,0.0020137022,0.0007278364,0.0008825797,0.00063219,0.00011528735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002499614,0.00074318144,0.0011471339,0.002897715,0.00056841876,0.0013240958,0.0019699642,0.0009016413,0.0013117202],"category_scores_gemma":[0.01417735,0.00043279587,0.0006798497,0.0014736995,0.00094656146,0.001896503,0.0016015811,0.0011976492,0.0008883948],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030810258,0.00013089452,0.035593446,0.0001742896,0.00040525958,0.00020217041,0.00036254225,0.10714443,0.015777616,0.040645055,0.004774037,0.7944821],"study_design_scores_gemma":[0.000053976153,0.00010300178,0.008707779,0.000036564474,0.00005918834,0.0003378774,0.000035911286,0.9516703,0.008568009,0.02241548,0.0078563085,0.00015561159],"about_ca_topic_score_codex":0.0030870084,"about_ca_topic_score_gemma":0.002442614,"teacher_disagreement_score":0.0030870084,"about_ca_system_score_codex":0.00045862776,"about_ca_system_score_gemma":0.0009722206,"threshold_uncertainty_score":0.013219357},"labels":[],"label_agreement":null},{"id":"W2012533198","doi":"10.1086/511330","title":"Infrared Photometric Analysis of White Dwarfs from the Two Micron All Sky Survey and the<i>Spitzer Space Telescope</i>","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Spitzer Space Telescope; Photometry (optics); Astrophysics; Stars; Sky; Astronomy; Infrared; Infrared excess; Brown dwarf; Infrared telescope; Telescope","score_opus":0.011571262564726945,"score_gpt":0.24250903255318354,"score_spread":0.2309377699884566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012533198","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86003894,0.06361572,0.019787619,0.00091880973,0.0003293503,0.000120447956,0.022209205,0.0007163181,0.032263633],"genre_scores_gemma":[0.8655429,0.03903405,0.018763509,0.00048645635,0.00055163435,0.000066853536,0.06802597,0.00017073292,0.0073579308],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972826,0.000022469085,0.000029920962,0.00005705657,0.00013975083,0.00002244437],"domain_scores_gemma":[0.9994686,0.000050731134,0.00019707868,0.000055771685,0.00018325064,0.00004462254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005807835,0.00037318107,0.00020779869,0.0038966122,0.00021326015,0.0004275214,0.00020613924,0.00011755556,0.00059982843],"category_scores_gemma":[0.0007542051,0.00008945991,0.0002912945,0.0025468257,0.0001436126,0.0003271455,0.0003555847,0.00013130083,0.0004528694],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000081573584,0.00005631447,0.7215286,0.0010294628,0.00029279606,0.00052014744,0.00045861193,0.00095061224,0.020336585,0.0015146735,0.01426012,0.23897055],"study_design_scores_gemma":[0.000001819592,0.00002774569,0.9591953,0.00005002275,0.000044677643,0.00047495286,0.00008496726,0.00017087877,0.0014468712,0.00029027264,0.038206555,0.0000059928316],"about_ca_topic_score_codex":0.005065208,"about_ca_topic_score_gemma":0.009905052,"teacher_disagreement_score":0.005065208,"about_ca_system_score_codex":0.000319972,"about_ca_system_score_gemma":0.00033661438,"threshold_uncertainty_score":0.010071456},"labels":[],"label_agreement":null},{"id":"W2012540188","doi":"10.1086/339505","title":"Three‐dimensional Simulations of the Gravitational Collapse of Logatropic Molecular Cloud Cores","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Protostar; Gravitational collapse; Hydrostatic equilibrium; Molecular cloud; Accretion (finance); Star formation; Gravitation","score_opus":0.01278811346106868,"score_gpt":0.2342865491937493,"score_spread":0.22149843573268063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012540188","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889098,0.00011041577,0.001919749,0.00030398802,0.000033728455,0.000052851403,0.00077024725,0.000146992,0.0077523603],"genre_scores_gemma":[0.995106,0.00008820387,0.002480359,0.0001260451,0.000018688286,0.000074563606,0.00089728663,0.000054945,0.0011539318],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998301,0.00003641236,0.0000081203725,0.000020978889,0.00003490959,0.00006941164],"domain_scores_gemma":[0.99877864,0.0005637313,0.00013065992,0.00004728765,0.00015140866,0.00032831583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003889813,0.000588078,0.0006321974,0.00053942716,0.001050617,0.0009367597,0.0013714338,0.0012825704,0.0025667897],"category_scores_gemma":[0.0022151214,0.00048076973,0.0006829434,0.00071954983,0.0011953908,0.00054693007,0.0008397116,0.0012937697,0.0001945093],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002513164,0.00020641282,0.0073134177,0.00003209275,0.00006188813,0.00020624595,0.00011023622,0.9872,0.0010184849,0.0019274337,0.00060084113,0.0010715488],"study_design_scores_gemma":[0.000072515824,0.000046300447,0.0024155409,0.000005365025,0.000008162475,0.000013954995,0.000057263514,0.9964399,0.00022189801,0.00046758784,0.00024171804,0.000009732119],"about_ca_topic_score_codex":0.06721392,"about_ca_topic_score_gemma":0.043558195,"teacher_disagreement_score":0.06721392,"about_ca_system_score_codex":0.0019912773,"about_ca_system_score_gemma":0.0017980087,"threshold_uncertainty_score":0.13364542},"labels":[],"label_agreement":null},{"id":"W2012578543","doi":"10.1086/498066","title":"Accretion-powered Stellar Winds as a Solution to the Stellar Angular Momentum Problem","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":355,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Accretion (finance); Angular momentum; T Tauri star; Astrophysics; Stars; Astronomy; Outflow; Stellar rotation; Stellar wind; Classical mechanics; Meteorology","score_opus":0.008523380223156367,"score_gpt":0.23738022531148115,"score_spread":0.22885684508832477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012578543","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.36184084,0.013412613,0.45650753,0.016606351,0.003539338,0.00009434782,0.00029755835,0.00082231115,0.14687903],"genre_scores_gemma":[0.91156286,0.004402811,0.05154499,0.0006363257,0.0016295398,0.00006299714,0.00012497915,0.00010402631,0.029931499],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99984765,0.00005363524,0.000009012299,0.000021065987,0.000038008748,0.000030585776],"domain_scores_gemma":[0.9997323,0.000084596664,0.00006308011,0.00003787389,0.000043223452,0.00003894266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043997858,0.00029762997,0.0003983775,0.00039494215,0.0007364647,0.0017526497,0.0007617852,0.0014281649,0.0037542025],"category_scores_gemma":[0.0020311698,0.00027402616,0.000436241,0.000322641,0.00085342576,0.0015336054,0.0011184168,0.000920946,0.0006901878],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012004957,0.000041084997,0.0026598715,0.00009257808,0.00005747175,0.00054575666,0.0001678172,0.07057888,0.00319427,0.8838372,0.0049699526,0.03373501],"study_design_scores_gemma":[0.00015111602,0.00006300895,0.0015056485,0.00005472621,0.000023825261,0.00047377063,0.00011847394,0.2348872,0.0007011414,0.7339888,0.027998837,0.000033361768],"about_ca_topic_score_codex":0.0011855797,"about_ca_topic_score_gemma":0.0012819341,"teacher_disagreement_score":0.0037542025,"about_ca_system_score_codex":0.0004423332,"about_ca_system_score_gemma":0.0005784654,"threshold_uncertainty_score":0.012559056},"labels":[],"label_agreement":null},{"id":"W2012813094","doi":"10.1088/0004-637x/706/1/348","title":"SIMULTANEOUS MULTI-WAVELENGTH OBSERVATIONS OF Sgr A* DURING 2007 APRIL 1-11","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Flare; Millimeter; Wavelength; Flux (metallurgy); Scattering; Light curve; Compton scattering; Photon","score_opus":0.020460054541675564,"score_gpt":0.24186028374889781,"score_spread":0.22140022920722224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012813094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99776864,0.000082676655,0.00028684546,0.000038206865,0.000009638923,0.000011270751,0.0009284698,0.000059398495,0.0008149209],"genre_scores_gemma":[0.99454534,0.000096670985,0.0018478367,0.000060664373,0.00003927211,0.000017951297,0.0028595587,0.00001722015,0.00051546574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981385,0.000014429914,0.000010308189,0.000066219414,0.000059113634,0.00003619003],"domain_scores_gemma":[0.99959177,0.000031878437,0.0001545722,0.000038094015,0.00006746271,0.000116307725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002485266,0.00028330286,0.0003602947,0.00085255527,0.0005000007,0.00048062307,0.000338345,0.0003309781,0.00053504313],"category_scores_gemma":[0.0002840301,0.0002254931,0.0002921325,0.00048666832,0.00016785956,0.00038533335,0.00072746194,0.00045622542,0.00021287517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082797173,0.00037924686,0.8099278,0.000105083855,0.00039678856,0.00066287885,0.00073777116,0.0014241234,0.15562317,0.00024126512,0.002376208,0.02729768],"study_design_scores_gemma":[0.000009490225,0.00012392522,0.9954265,0.0000038238622,0.00002739146,0.00021179675,0.00008216986,0.0007715594,0.0022617716,0.00003090753,0.0010428238,0.000007947595],"about_ca_topic_score_codex":0.0047636605,"about_ca_topic_score_gemma":0.019704616,"teacher_disagreement_score":0.0047636605,"about_ca_system_score_codex":0.00035673723,"about_ca_system_score_gemma":0.0002794546,"threshold_uncertainty_score":0.009471893},"labels":[],"label_agreement":null},{"id":"W2012826046","doi":"10.1086/309484","title":"The MACHO Project: Microlensing Optical Depth toward the Galactic Bulge from Difference Image Analysis","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gravitational microlensing; Bulge; Physics; Astrophysics; Photometry (optics); Stars; Initial mass function; Light curve; Population; Mass distribution; Optical depth; Astronomy; Galaxy; Star formation","score_opus":0.012455301225290172,"score_gpt":0.23778953049687646,"score_spread":0.22533422927158628,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012826046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83172446,0.0032503458,0.11524475,0.0009906549,0.00019624145,0.00033068613,0.019080373,0.011111047,0.01807148],"genre_scores_gemma":[0.8608215,0.00049205887,0.111347996,0.00016205318,0.00017090439,0.00013518051,0.022157472,0.00091620977,0.0037966173],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9996592,0.00004597714,0.000010777203,0.000066002256,0.00014068643,0.00007736362],"domain_scores_gemma":[0.99954873,0.00005124579,0.000059853694,0.0001144077,0.000098221986,0.00012756664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006619311,0.00042169465,0.0003832388,0.0022748194,0.0002856203,0.0014285892,0.0006958668,0.00047812724,0.0020053717],"category_scores_gemma":[0.001215971,0.00028764666,0.00036171314,0.0010997589,0.00023158791,0.00076779636,0.0023813546,0.00051694224,0.0009406073],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012553553,0.00037823967,0.14396651,0.00036574202,0.00053017336,0.00045415945,0.0011138009,0.0079728,0.13456888,0.004740179,0.034860685,0.6697934],"study_design_scores_gemma":[0.00026570068,0.0001933277,0.723114,0.00009137869,0.00020930338,0.0009363417,0.001021154,0.17950317,0.041165598,0.00935857,0.044010144,0.00013129914],"about_ca_topic_score_codex":0.0051197684,"about_ca_topic_score_gemma":0.008840129,"teacher_disagreement_score":0.0051197684,"about_ca_system_score_codex":0.00035616892,"about_ca_system_score_gemma":0.0003579333,"threshold_uncertainty_score":0.010179937},"labels":[],"label_agreement":null},{"id":"W2012851284","doi":"10.1086/421447","title":"On the Driving Mechanism and the Coexistence of Variable and Nonvariable Stars in the Domain of the Pulsating PG 1159 Stars","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Stars; Astrophysics; Variable star; Homogeneous; Astronomy; Statistical physics","score_opus":0.007869904909344137,"score_gpt":0.20301803242855757,"score_spread":0.19514812751921343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012851284","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99731064,0.00023804045,0.0007584703,0.00014195094,0.0000024201488,0.000002003076,0.00002835098,0.000010123479,0.0015080575],"genre_scores_gemma":[0.99969196,0.00008169228,0.000111854504,0.000008268839,0.000005228208,5.577207e-7,0.000024887,0.000002014276,0.00007360931],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986684,0.000030330051,0.000008938347,0.00003904381,0.000020001242,0.000034744106],"domain_scores_gemma":[0.9988538,0.000533824,0.00029312618,0.00012641391,0.000047148453,0.00014562259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004891684,0.00022429357,0.0002926083,0.0007874588,0.00054571574,0.0010671858,0.00044918995,0.0004521779,0.0014345079],"category_scores_gemma":[0.0019365933,0.000101308506,0.00018527414,0.00064483413,0.00089010166,0.00093816075,0.0011172513,0.00026628614,0.00022219995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064092287,0.00007690117,0.9117309,0.000114986564,0.000072706775,0.0019552226,0.0016139604,0.0049234703,0.027229171,0.026791455,0.0002740196,0.024576286],"study_design_scores_gemma":[0.00004701131,0.00025193224,0.8937889,0.000043354554,0.0001156793,0.0037670557,0.0025697614,0.041107006,0.008883603,0.046577033,0.002814497,0.000034188146],"about_ca_topic_score_codex":0.0007569419,"about_ca_topic_score_gemma":0.000782231,"teacher_disagreement_score":0.0014345079,"about_ca_system_score_codex":0.00025911402,"about_ca_system_score_gemma":0.00013387982,"threshold_uncertainty_score":0.004798889},"labels":[],"label_agreement":null},{"id":"W2012874460","doi":"10.1086/323208","title":"Profiles of the λ6196 and λ6379 Diffuse Interstellar Bands","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Stars; Moment of inertia; Interstellar medium; Line (geometry); Geometry; Galaxy; Classical mechanics","score_opus":0.007166966633104576,"score_gpt":0.22967240745396902,"score_spread":0.22250544082086446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012874460","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985446,0.000034566146,0.00067780673,0.000006348438,0.0000011300215,0.0000018344422,0.00013905973,0.000023139983,0.000571601],"genre_scores_gemma":[0.99809927,0.000023479186,0.00087952334,0.000006404294,0.0000011987186,0.000002788391,0.00050500344,0.00001867062,0.0004636798],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999915,0.0000034113614,0.0000040584155,0.000032423955,0.000026227865,0.000018890682],"domain_scores_gemma":[0.99977905,0.000022367387,0.00004631074,0.000022296297,0.00006107785,0.00006893479],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014245155,0.0001755821,0.0001500357,0.0004474858,0.0003182801,0.0003370495,0.00020636305,0.0002453875,0.0011933288],"category_scores_gemma":[0.00031970916,0.00012136516,0.0001948986,0.00046527272,0.00014520397,0.0002176546,0.00032510806,0.00030277675,0.0005287187],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039649167,0.000097351214,0.2863395,0.00006204334,0.00007342437,0.0002302571,0.0006467097,0.004453868,0.68203974,0.0008787085,0.00026809616,0.024513721],"study_design_scores_gemma":[0.000013903069,0.00014659738,0.90416104,0.000009058848,0.00003633211,0.00037272938,0.00037571992,0.01242682,0.07953219,0.0004849241,0.0024174964,0.000023172675],"about_ca_topic_score_codex":0.0011791914,"about_ca_topic_score_gemma":0.0013817647,"teacher_disagreement_score":0.0011933288,"about_ca_system_score_codex":0.0002665701,"about_ca_system_score_gemma":0.000068390254,"threshold_uncertainty_score":0.003992021},"labels":[],"label_agreement":null},{"id":"W2012881615","doi":"10.1088/0004-637x/697/2/1032","title":"THE THIRD SIGNATURE OF STELLAR GRANULATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Granulation; Astrophysics; Photosphere; Line (geometry); Effective temperature; Spectral line; Stars; Astronomy; Geometry","score_opus":0.0071927698021355254,"score_gpt":0.2183688529837712,"score_spread":0.2111760831816357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012881615","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98868656,0.0000893461,0.0041954084,0.00004677623,0.000009647768,0.000007523649,0.00021152002,0.00033120587,0.0064219623],"genre_scores_gemma":[0.9981343,0.000020665384,0.0012613025,0.000018097355,0.0000033966814,0.0000026864604,0.000111750545,0.000025257825,0.00042239059],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998609,0.000011569437,0.000009658094,0.00003365799,0.000052825406,0.00003144401],"domain_scores_gemma":[0.99879885,0.00016770813,0.00048320473,0.00020385325,0.00017374843,0.00017270651],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013707163,0.00013638586,0.00019496755,0.00091166946,0.0002829541,0.0006417968,0.00014818918,0.00018184083,0.0024661066],"category_scores_gemma":[0.0008910975,0.00010019338,0.00017513984,0.00047538872,0.0005563672,0.0002628521,0.00087872794,0.0003374723,0.0004856678],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013463981,0.00007407694,0.3725156,0.00024628532,0.00010888605,0.00049231073,0.0014519615,0.002232003,0.50475115,0.006886827,0.0015122832,0.10838221],"study_design_scores_gemma":[0.000027976337,0.0002345553,0.917309,0.000021884996,0.000032136326,0.0030091456,0.00036113878,0.004973009,0.06374971,0.0036084894,0.006632649,0.000040290226],"about_ca_topic_score_codex":0.00047219073,"about_ca_topic_score_gemma":0.00047133607,"teacher_disagreement_score":0.0024661066,"about_ca_system_score_codex":0.00018797173,"about_ca_system_score_gemma":0.00013591589,"threshold_uncertainty_score":0.0082499385},"labels":[],"label_agreement":null},{"id":"W2012953163","doi":"10.1088/0004-637x/767/2/133","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. IV. NGC 4216: A BOMBARDED SPIRAL IN THE VIRGO CLUSTER","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Waterloo; National Research Council Canada","funders":"","keywords":"Virgo Cluster; Physics; Astrophysics; Dwarf galaxy; Astronomy; Cluster (spacecraft); Surface brightness; Galaxy; Spiral galaxy; Fornax Cluster; Stars; Star formation; Galaxy cluster","score_opus":0.02070742335959473,"score_gpt":0.22687151206214914,"score_spread":0.20616408870255443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2012953163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9669717,0.00060063734,0.0003527774,0.00060888234,0.000060984443,0.0001050575,0.020180127,0.000208289,0.010911555],"genre_scores_gemma":[0.9508484,0.00040398276,0.0015663722,0.00025104178,0.00005289734,0.00007511771,0.031479873,0.00009238517,0.015229858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998116,0.000019458737,0.000009918364,0.00003546538,0.000057117788,0.00006658103],"domain_scores_gemma":[0.9993685,0.000024798741,0.000101666286,0.00006231531,0.00008295569,0.0003598709],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041839108,0.00036972263,0.00037664972,0.0019638557,0.00087643723,0.0005428189,0.0006092155,0.0005343021,0.0037400953],"category_scores_gemma":[0.00062658667,0.00022503773,0.00026068653,0.0020201798,0.000309022,0.000309861,0.0014930044,0.00030244008,0.0015440925],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081895804,0.00014110577,0.9167284,0.000091316295,0.000075747776,0.00092210976,0.00097261596,0.00053534715,0.012565376,0.0006926298,0.025041157,0.04141526],"study_design_scores_gemma":[0.000023872448,0.00007523496,0.98582166,0.000018080014,0.000026815569,0.0002882934,0.0002884774,0.00019665547,0.00054617535,0.00012734503,0.012579123,0.000008193642],"about_ca_topic_score_codex":0.08086186,"about_ca_topic_score_gemma":0.123966284,"teacher_disagreement_score":0.08086186,"about_ca_system_score_codex":0.0014679933,"about_ca_system_score_gemma":0.0009300294,"threshold_uncertainty_score":0.1607824},"labels":[],"label_agreement":null},{"id":"W2013036784","doi":"10.1086/587543","title":"Global Models for the Evolution of Embedded, Accreting Protostellar Disks","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":191,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Angular momentum; Dimensionless quantity; Accretion (finance); Gravitational instability; Protostar; Stars; Stellar evolution; Star formation","score_opus":0.020152224918833204,"score_gpt":0.2606017787524886,"score_spread":0.24044955383365538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013036784","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3699958,0.007359723,0.5722662,0.0020321156,0.00017158662,0.00018044087,0.002413501,0.0014472128,0.044133417],"genre_scores_gemma":[0.9358201,0.003991581,0.04810622,0.00017966036,0.00013665168,0.0003251802,0.0009955539,0.00033437466,0.010110677],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998932,0.0000330858,0.000005750497,0.00003303926,0.000019319954,0.000015625303],"domain_scores_gemma":[0.99974626,0.0000828395,0.00006426922,0.000039003266,0.000029598723,0.000038140985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030660475,0.0008339035,0.00054269005,0.00058971415,0.00046934278,0.0016260195,0.0018377806,0.001058268,0.0021228974],"category_scores_gemma":[0.0011396962,0.0003968789,0.00071594334,0.00077197264,0.0009590069,0.002219338,0.00095976295,0.0007394218,0.00063256116],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002896314,0.0000275442,0.0064573595,0.00006327615,0.00006296818,0.00010931345,0.00021204246,0.8846922,0.0013867302,0.09903779,0.00094346364,0.006978426],"study_design_scores_gemma":[0.000036958405,0.000040573414,0.0038699459,0.000017076856,0.000049111764,0.00016002075,0.00008642743,0.86504805,0.00021882632,0.12355613,0.0068987566,0.000018038974],"about_ca_topic_score_codex":0.0038664183,"about_ca_topic_score_gemma":0.0038612445,"teacher_disagreement_score":0.0038664183,"about_ca_system_score_codex":0.0010312619,"about_ca_system_score_gemma":0.00044441488,"threshold_uncertainty_score":0.007687807},"labels":[],"label_agreement":null},{"id":"W2013101677","doi":"10.1086/322347","title":"Dynamics of the Globular Cluster System Associated with M87 (NGC 4486). II. Analysis","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":251,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Queen's University; University of Waterloo; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Photometry (optics); Star cluster; Cluster (spacecraft); Galaxy; Astronomy; Galaxy cluster; Virgo Cluster; Stars","score_opus":0.0037281913447040856,"score_gpt":0.18411868436699963,"score_spread":0.18039049302229554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013101677","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960628,0.00008392016,0.00092892844,0.000038099737,0.0000019140537,0.000022201264,0.0011878076,0.000021599457,0.0016525642],"genre_scores_gemma":[0.9950257,0.00008720099,0.001528784,0.000010143646,0.0000051053394,0.000017457704,0.0023732993,0.000010230276,0.00094207755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988866,0.000012008855,0.000005606879,0.000035460536,0.000030208892,0.00002809341],"domain_scores_gemma":[0.9996915,0.00005948119,0.00008551922,0.00002758511,0.000086016116,0.0000498338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013740036,0.0001516599,0.00023739682,0.0014158019,0.00046274095,0.0005709115,0.00026074867,0.00015343301,0.001581494],"category_scores_gemma":[0.00069435313,0.000093019364,0.00024825588,0.00092416763,0.0002358343,0.00022332331,0.00056937797,0.00017898921,0.00036448875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007972701,0.000038564423,0.962141,0.000037924518,0.000040026684,0.00021275949,0.0005083818,0.0075358036,0.006539179,0.0023841185,0.0009724453,0.01951019],"study_design_scores_gemma":[0.0000028057505,0.000022379367,0.9778862,0.0000050040862,0.000014505979,0.00018473953,0.00022049529,0.01895494,0.00083560223,0.00037480053,0.0014901145,0.000008392039],"about_ca_topic_score_codex":0.030872608,"about_ca_topic_score_gemma":0.0298981,"teacher_disagreement_score":0.030872608,"about_ca_system_score_codex":0.0009683882,"about_ca_system_score_gemma":0.00037647615,"threshold_uncertainty_score":0.06138581},"labels":[],"label_agreement":null},{"id":"W2013125620","doi":"10.1086/320555","title":"Galaxy Groups at Intermediate Redshift","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Velocity dispersion; Galaxy group; Galaxy; Brightest cluster galaxy; Galaxy cluster; Dark matter; Lenticular galaxy; Radio galaxy; Redshift","score_opus":0.007457874669290087,"score_gpt":0.21142608525162174,"score_spread":0.20396821058233164,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013125620","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.974718,0.0004583088,0.00064228266,0.00011784124,0.00001712948,0.000028704597,0.004133707,0.00021124538,0.01967277],"genre_scores_gemma":[0.99511623,0.00006989894,0.00028503063,0.000025805522,0.000009682665,0.000009123129,0.002905249,0.00001331754,0.0015656],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995161,0.00003371432,0.000017241278,0.00009189567,0.00009510109,0.0002458517],"domain_scores_gemma":[0.99904007,0.00006470149,0.0002480775,0.00012160732,0.00010406377,0.00042144462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029243343,0.00026975136,0.00032538865,0.0043690167,0.0005718643,0.001477077,0.0003627851,0.00025236906,0.011164137],"category_scores_gemma":[0.001288064,0.00010858552,0.00032782735,0.0020496899,0.00031026007,0.00045659067,0.0014001509,0.0002994447,0.0015901764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029860553,0.00004189944,0.9568752,0.000052172254,0.00011565134,0.00021269385,0.0012489045,0.00040758372,0.00354508,0.008935645,0.003194081,0.025072519],"study_design_scores_gemma":[0.000004807145,0.00002088487,0.99424875,0.000009950107,0.0000114975455,0.000084584935,0.0003043419,0.00019935926,0.00011993476,0.0009306514,0.0040591424,0.000006023039],"about_ca_topic_score_codex":0.0128425965,"about_ca_topic_score_gemma":0.010404714,"teacher_disagreement_score":0.0128425965,"about_ca_system_score_codex":0.0005144655,"about_ca_system_score_gemma":0.00021231025,"threshold_uncertainty_score":0.037347734},"labels":[],"label_agreement":null},{"id":"W2013224022","doi":"10.1088/0004-637x/748/2/118","title":"SEARCHES FOR PERIODIC NEUTRINO EMISSION FROM BINARY SYSTEMS WITH 22 AND 40 STRINGS OF ICECUBE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Marsden Fund; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Vetenskapsrådet; Fonds Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; Belgian Federal Science Policy Office; Bundesministerium für Bildung und Forschung; Office of Polar Programs; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Knut och Alice Wallenbergs Stiftelse; University of Oxford; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Neutrino; Flux (metallurgy); String (physics); Binary number; Neutrino detector; Photon; Sensitivity (control systems); Measurements of neutrino speed; Astrophysics; Neutrino oscillation; Particle physics; Nuclear physics; Solar neutrino; Theoretical physics; Optics","score_opus":0.014412318017634623,"score_gpt":0.22959058820544045,"score_spread":0.21517827018780583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013224022","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99725634,0.00012790534,0.00025957177,0.000019176116,0.000004606356,0.0000075247303,0.0005716663,0.000018542842,0.001734768],"genre_scores_gemma":[0.993292,0.00009801068,0.0012951008,0.000023251574,0.000020658263,0.000016436623,0.0047587515,0.00001733605,0.0004785861],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992686,0.0001646392,0.00004044828,0.0001615563,0.00020508135,0.00015954838],"domain_scores_gemma":[0.9978156,0.0006516724,0.00088785676,0.00027438445,0.00016322517,0.00020734237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010607985,0.00027368305,0.0004947371,0.0016136704,0.00062372495,0.0011239579,0.00033650946,0.0003748989,0.0015899129],"category_scores_gemma":[0.0025757772,0.00024163033,0.00033546446,0.0019814076,0.0003496922,0.0005529425,0.00084001163,0.00024405544,0.00020230489],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018623186,0.00012167944,0.94409287,0.000095813724,0.00034404782,0.00087975536,0.00032825593,0.0037576396,0.023086153,0.0016873013,0.0013667076,0.022377431],"study_design_scores_gemma":[0.000049315706,0.00016621797,0.98053104,0.000023655099,0.000080450685,0.00081649056,0.00022860989,0.005855029,0.007226587,0.00069295015,0.0043073143,0.000022227505],"about_ca_topic_score_codex":0.0023054576,"about_ca_topic_score_gemma":0.0038957237,"teacher_disagreement_score":0.0023054576,"about_ca_system_score_codex":0.0005302737,"about_ca_system_score_gemma":0.00034776414,"threshold_uncertainty_score":0.0056101084},"labels":[],"label_agreement":null},{"id":"W2013296434","doi":"10.1088/0004-637x/773/2/169","title":"ENERGY CONSERVATION AND GRAVITY WAVES IN SOUND-PROOF TREATMENTS OF STELLAR INTERIORS. II. LAGRANGIAN CONSTRAINED ANALYSIS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Radiative transfer; Convection; Stellar atmosphere; Stratified flows; Stratified flow; Buoyancy; Supernova; Gravitational wave; Radiative cooling","score_opus":0.005884541654282148,"score_gpt":0.21398749086732866,"score_spread":0.2081029492130465,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013296434","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.027058925,0.0062778657,0.91183496,0.005018735,0.0005342158,0.00008379468,0.00036048377,0.00015095736,0.04868012],"genre_scores_gemma":[0.6169545,0.00924427,0.32252115,0.00226893,0.0016445442,0.0005476821,0.00063567597,0.0007154059,0.045467705],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997774,0.000097290635,0.000013759482,0.000022578539,0.00006483971,0.000024231786],"domain_scores_gemma":[0.99963593,0.00015707052,0.0000694318,0.00005046263,0.00005350792,0.000033530574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00086855976,0.0006269389,0.00043801195,0.0008710648,0.000530019,0.0011381941,0.0012396548,0.0012096963,0.003809511],"category_scores_gemma":[0.0018375638,0.00032325738,0.0009893728,0.00058087707,0.001932201,0.0021103334,0.0017161751,0.0018059184,0.0007244912],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000046315154,0.000013600713,0.0004044734,0.000060476188,0.0000110787505,0.0000644844,0.00014908236,0.03649291,0.0007566794,0.95079374,0.0025369418,0.008711852],"study_design_scores_gemma":[0.0000044529615,0.000012246759,0.00041899455,0.000049780076,0.000005328074,0.000032280568,0.00005824594,0.22969447,0.00024507332,0.7556508,0.013817056,0.000011265912],"about_ca_topic_score_codex":0.00338125,"about_ca_topic_score_gemma":0.00284985,"teacher_disagreement_score":0.003809511,"about_ca_system_score_codex":0.001000199,"about_ca_system_score_gemma":0.00074594835,"threshold_uncertainty_score":0.012744069},"labels":[],"label_agreement":null},{"id":"W2013433349","doi":"10.1088/0004-637x/745/2/146","title":"NONTHERMAL RADIATION FROM COSMIC-RAY MODIFIED SHOCKS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Cosmic ray; Radiation; Astrophysics; Astronomy; Background radiation; COSMIC cancer database; Space radiation; Nuclear physics","score_opus":0.010018076743229047,"score_gpt":0.21910944823737002,"score_spread":0.20909137149414098,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013433349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9747312,0.00028931408,0.015505181,0.000102525024,0.000035259618,0.00004860378,0.0004266754,0.00019506848,0.008666222],"genre_scores_gemma":[0.9963887,0.00015432411,0.0019403988,0.000028413211,0.000011704891,0.00002080675,0.00025230215,0.000049986396,0.0011534858],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998739,0.00002488607,0.00000832902,0.000020070955,0.00003649799,0.000036349975],"domain_scores_gemma":[0.9996456,0.00010376641,0.00007222926,0.0000388367,0.0000818706,0.00005775063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022594784,0.00063628674,0.00043576912,0.0004994477,0.0003100859,0.0009255511,0.0008537478,0.0007069289,0.0010742581],"category_scores_gemma":[0.001587714,0.00035206048,0.0007371862,0.00078657386,0.0005028229,0.00051852234,0.00055184134,0.00040205187,0.00017401109],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101307356,0.00003871222,0.004924425,0.000036977384,0.00004437599,0.0002713231,0.000044470635,0.98709494,0.003259106,0.0026750755,0.00013103921,0.001378267],"study_design_scores_gemma":[0.000062592786,0.000052499017,0.0042133788,0.000004871657,0.000019419303,0.00006671545,0.000034203003,0.99287134,0.0015678171,0.0008349399,0.00025882135,0.000013472567],"about_ca_topic_score_codex":0.012790073,"about_ca_topic_score_gemma":0.0043699066,"teacher_disagreement_score":0.012790073,"about_ca_system_score_codex":0.0007666156,"about_ca_system_score_gemma":0.0006595845,"threshold_uncertainty_score":0.025431275},"labels":[],"label_agreement":null},{"id":"W2013448060","doi":"10.1088/0004-637x/766/2/120","title":"THE THREE-DIMENSIONAL STRUCTURE OF THE M31 SATELLITE SYSTEM; STRONG EVIDENCE FOR AN INHOMOGENEOUS DISTRIBUTION OF SATELLITES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Milky Way; Satellite; Asymmetry; Satellite galaxy; Perpendicular; Planar","score_opus":0.013578659413959655,"score_gpt":0.2303297428976506,"score_spread":0.21675108348369093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013448060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99809533,0.00012029915,0.00055930566,0.000026125415,8.828265e-7,0.0000019222498,0.00015246429,0.000014785388,0.0010289132],"genre_scores_gemma":[0.9990227,0.0000509866,0.0006170191,0.000007710072,0.0000037912305,0.0000020388202,0.00019369031,0.0000059108756,0.000096094474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998863,0.000016467098,0.000007023409,0.000034236433,0.000032847078,0.000023099303],"domain_scores_gemma":[0.99922657,0.0001407059,0.0002746006,0.00010397854,0.00016098352,0.00009329131],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018122481,0.000091686576,0.00012335011,0.0016400637,0.00034904922,0.00062518066,0.00022363012,0.00016726633,0.0006727621],"category_scores_gemma":[0.000796262,0.00013306426,0.00011555096,0.0013046279,0.0004604097,0.00039036098,0.0005699685,0.00016270118,0.00028914792],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001055861,0.000017462917,0.90709573,0.00004665909,0.000055851182,0.00043336168,0.0009605902,0.002377291,0.073490724,0.0019305942,0.00043797624,0.013048295],"study_design_scores_gemma":[0.00000318713,0.000019739344,0.9914977,0.000005343056,0.000011718083,0.0004052731,0.00037916712,0.0039336197,0.0021823526,0.00040663878,0.0011439973,0.000011214259],"about_ca_topic_score_codex":0.0030559755,"about_ca_topic_score_gemma":0.0045476356,"teacher_disagreement_score":0.0030559755,"about_ca_system_score_codex":0.00025290402,"about_ca_system_score_gemma":0.00020533674,"threshold_uncertainty_score":0.0060763955},"labels":[],"label_agreement":null},{"id":"W2013533377","doi":"10.1086/528931","title":"Probing the Central Regions of Nearby Compact Elliptical Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Elliptical galaxy; Galaxy; Angular resolution (graph drawing); Angular diameter; Fundamental plane (elliptical galaxies); Hubble sequence; Lenticular galaxy; Galaxy group","score_opus":0.014556253128430533,"score_gpt":0.2160581075746627,"score_spread":0.20150185444623217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013533377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975249,0.0001526656,0.00050021376,0.00002528018,0.0000022474699,0.0000030633464,0.00017322837,0.00004493855,0.0015734185],"genre_scores_gemma":[0.9984774,0.000048573613,0.0008901698,0.000012581571,0.000005089687,0.000001882755,0.00019053301,0.000004768654,0.00036900333],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999434,0.000003170097,0.0000012729927,0.00002795218,0.000008462585,0.000015741542],"domain_scores_gemma":[0.9997893,0.000024881923,0.0000702241,0.00003540693,0.000026900721,0.00005324697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013909348,0.00011052462,0.00012346673,0.00035226578,0.00026742645,0.0002875696,0.000184239,0.00018445837,0.0009683957],"category_scores_gemma":[0.00026038694,0.00013994693,0.00009603682,0.00026697502,0.00013647172,0.00029847393,0.00025444347,0.00013209085,0.000251494],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044618224,0.00011015784,0.35204613,0.000060172595,0.000056217476,0.00019236031,0.0006990619,0.00067691243,0.6152523,0.0006809796,0.0007184731,0.029061168],"study_design_scores_gemma":[0.000013807975,0.000067858244,0.97773963,0.0000071506165,0.000024049954,0.00029519683,0.00017474094,0.0013158942,0.0177466,0.00027256343,0.002334774,0.000007910951],"about_ca_topic_score_codex":0.0022504828,"about_ca_topic_score_gemma":0.0056190244,"teacher_disagreement_score":0.0022504828,"about_ca_system_score_codex":0.00023756777,"about_ca_system_score_gemma":0.00008242419,"threshold_uncertainty_score":0.004474759},"labels":[],"label_agreement":null},{"id":"W2013549053","doi":"10.1088/0004-637x/757/2/156","title":"MOLECULAR AND ATOMIC LINE SURVEYS OF GALAXIES. I. THE DENSE, STAR-FORMING GAS PHASE AS A BEACON","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Luminous infrared galaxy; Luminosity; Interstellar medium; Line (geometry); Astronomy; Redshift; Universe; Infrared; Atomic carbon; Submillimeter Array; Hydrogen","score_opus":0.009243407119003384,"score_gpt":0.238380612236241,"score_spread":0.22913720511723762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013549053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8974266,0.0039033897,0.04532861,0.00085351744,0.000051029954,0.00023329117,0.02780669,0.0009234095,0.023473432],"genre_scores_gemma":[0.9671786,0.0011110613,0.021703798,0.00020956444,0.00009471075,0.00009785428,0.0060731997,0.000026477977,0.0035046407],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963176,0.00013764389,0.0000146593475,0.00008561978,0.000085197134,0.000045061006],"domain_scores_gemma":[0.998735,0.00017286734,0.00048803314,0.00016403032,0.00018710498,0.00025296575],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071809784,0.000273244,0.00016847483,0.0015353888,0.00019990173,0.0005551981,0.0005118045,0.00047030274,0.0028389858],"category_scores_gemma":[0.0015698882,0.00016511173,0.0002277126,0.0017270664,0.0002645643,0.001041693,0.00045469392,0.00020356494,0.0009993598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013672955,0.00007645185,0.9400387,0.00013272176,0.00009161203,0.000040745086,0.00019618821,0.0059666983,0.0046791006,0.010364539,0.0030432236,0.035233334],"study_design_scores_gemma":[0.000026661713,0.00016930199,0.95407563,0.00004929648,0.000033292486,0.00015829878,0.00019733359,0.018672492,0.0011288909,0.003666881,0.021803591,0.000018260514],"about_ca_topic_score_codex":0.007926268,"about_ca_topic_score_gemma":0.010406542,"teacher_disagreement_score":0.007926268,"about_ca_system_score_codex":0.00049565005,"about_ca_system_score_gemma":0.00022646092,"threshold_uncertainty_score":0.015760243},"labels":[],"label_agreement":null},{"id":"W2013663756","doi":"10.1088/0004-637x/769/2/123","title":"PHOTOMETRIC VARIABILITY IN A WARM, STRONGLY MAGNETIC DQ WHITE DWARF, SDSS J103655.39+652252.2","year":2013,"lang":"fr","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"National Science Foundation","keywords":"Physics; Astrophysics; White dwarf; Amplitude; Photometry (optics); Stars; Optics","score_opus":0.009652000929641559,"score_gpt":0.21716557437118852,"score_spread":0.20751357344154697,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013663756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99886864,0.00008992967,0.00017165809,0.000021737862,0.000004571947,0.0000024721355,0.00022941035,0.000047833128,0.0005638687],"genre_scores_gemma":[0.998703,0.00002847098,0.00024043466,0.000022711365,0.000006915084,0.0000022689273,0.00082601793,0.000007633648,0.0001625121],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998921,0.000009535191,0.00001013385,0.00004258876,0.000024614703,0.000020957634],"domain_scores_gemma":[0.99981326,0.000013394596,0.00007277618,0.000016251885,0.00001798875,0.000066264285],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017028562,0.00024069312,0.00020371366,0.0005819937,0.0002879018,0.00043737923,0.00024685037,0.0002573124,0.00040672175],"category_scores_gemma":[0.00036228084,0.00010645029,0.00014758536,0.0006666518,0.0001832708,0.00014864333,0.0002900259,0.00015501815,0.00026808665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023401166,0.00013907651,0.88563436,0.00005743958,0.00009967495,0.0019070855,0.00067190186,0.003555193,0.084517606,0.00064000825,0.0025958286,0.01994786],"study_design_scores_gemma":[0.00001743734,0.000058683225,0.99014705,0.000005170725,0.000025650867,0.00066755415,0.00013132209,0.0036912193,0.0020536063,0.00015054905,0.003039507,0.00001227906],"about_ca_topic_score_codex":0.0074397763,"about_ca_topic_score_gemma":0.011969627,"teacher_disagreement_score":0.0074397763,"about_ca_system_score_codex":0.000488547,"about_ca_system_score_gemma":0.00008699979,"threshold_uncertainty_score":0.014792919},"labels":[],"label_agreement":null},{"id":"W2013798962","doi":"10.1086/521209","title":"The Thermal Structure of the Circumstellar Disk Surrounding the Classical Be Star γ Cassiopeiae","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Hydrostatic equilibrium; Astrophysics; Thermal; Envelope (radar); Radiative transfer; Radiative equilibrium; Circumstellar envelope; Hydrogen; Radiative cooling; Thermal equilibrium; Chemical composition; Star (game theory); Ion; Thermodynamics; Stars; Astronomy; Optics","score_opus":0.01096412930935745,"score_gpt":0.2428518626152405,"score_spread":0.23188773330588305,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013798962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99163604,0.000107720945,0.0017916657,0.00008354633,0.00000501114,0.000010090031,0.00026481805,0.00007081382,0.006030399],"genre_scores_gemma":[0.9976119,0.00008957949,0.0013542885,0.000020355381,0.0000050614312,0.000009026989,0.00030469502,0.000025018548,0.00057998236],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999167,0.0000088994275,0.0000038065841,0.00003207231,0.000015551917,0.000023059241],"domain_scores_gemma":[0.9997768,0.000071111186,0.000032849086,0.00003210182,0.00004832552,0.00003889124],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015195244,0.0003985091,0.00034531773,0.00033230855,0.00093535456,0.00089148304,0.0010018226,0.0005619014,0.001577043],"category_scores_gemma":[0.00082692906,0.0003474286,0.00034037887,0.0005368699,0.0005797885,0.0005653754,0.00043977922,0.0005645208,0.0002360838],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020401864,0.00007864104,0.057082757,0.000089569934,0.000112443944,0.00094670634,0.0004377649,0.9095974,0.017826624,0.007942472,0.0006695168,0.0050121853],"study_design_scores_gemma":[0.00013989657,0.00011100163,0.046519417,0.00002079111,0.00006952793,0.00024853667,0.00027242815,0.9406843,0.0065124095,0.0031912925,0.0021877475,0.000042568663],"about_ca_topic_score_codex":0.040645488,"about_ca_topic_score_gemma":0.016743274,"teacher_disagreement_score":0.040645488,"about_ca_system_score_codex":0.0018041845,"about_ca_system_score_gemma":0.00077149976,"threshold_uncertainty_score":0.08081782},"labels":[],"label_agreement":null},{"id":"W2013878813","doi":"10.1088/0004-637x/703/2/1352","title":"THE DYNAMICS OF RADIATION-PRESSURE-DOMINATED H II REGIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":276,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Radiation pressure; Radiation; H II region; Star formation; Dynamics (music); Star cluster; High pressure","score_opus":0.005585684884082261,"score_gpt":0.2307107214673345,"score_spread":0.22512503658325225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013878813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99511755,0.0002278948,0.0010883529,0.000047231413,0.0000031730526,0.000013068057,0.00013719908,0.000020302743,0.00334519],"genre_scores_gemma":[0.9989471,0.00009318048,0.00035598935,0.000015007664,0.0000048802735,0.000005839753,0.00008686189,0.000005782605,0.0004854102],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999393,0.0000067691376,0.000002197001,0.000018247845,0.000008935159,0.000024543479],"domain_scores_gemma":[0.9995579,0.000083365616,0.00013290303,0.000017876479,0.000054285956,0.00015365078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019276842,0.00019536317,0.0001850284,0.00030981997,0.00034419957,0.00068821077,0.0004131591,0.0002834828,0.0016069363],"category_scores_gemma":[0.0007598968,0.0001740554,0.00015245214,0.00020302975,0.0003238966,0.0005428373,0.00047968572,0.00024810564,0.0002575984],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001005282,0.00020691917,0.458811,0.00016376797,0.00018673322,0.0016865018,0.00196882,0.056168154,0.43562263,0.021007907,0.0012370393,0.021935204],"study_design_scores_gemma":[0.00010740527,0.00053195585,0.7991592,0.00003209164,0.00009250889,0.0013285041,0.0011777282,0.122555256,0.058344036,0.010473758,0.006128686,0.00006886147],"about_ca_topic_score_codex":0.002245234,"about_ca_topic_score_gemma":0.0013409595,"teacher_disagreement_score":0.002245234,"about_ca_system_score_codex":0.00052711176,"about_ca_system_score_gemma":0.00016782212,"threshold_uncertainty_score":0.005375743},"labels":[],"label_agreement":null},{"id":"W2013910693","doi":"10.1088/0004-637x/771/1/29","title":"THE STELLAR INITIAL MASS FUNCTION OF ULTRA-FAINT DWARF GALAXIES: EVIDENCE FOR IMF VARIATIONS WITH GALACTIC ENVIRONMENT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":204,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Initial mass function; Galaxy; Luminosity function; Stars; Luminosity; Stellar mass; Dwarf galaxy; Star formation","score_opus":0.013472636280617647,"score_gpt":0.22152486610786104,"score_spread":0.2080522298272434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013910693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988067,0.00016457017,0.00006735254,0.00002823261,0.0000012214581,0.0000012414234,0.00017147664,0.000005740585,0.00075342087],"genre_scores_gemma":[0.99943525,0.0000502885,0.000056237473,0.000007817556,0.0000020497316,9.578539e-7,0.00019716215,0.0000022712234,0.00024789345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999474,0.000009223932,0.000004033167,0.000014146281,0.000010331683,0.000014755806],"domain_scores_gemma":[0.9992586,0.00012366677,0.00023218922,0.00006240569,0.00013584613,0.00018734844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023690751,0.00007664089,0.00011424694,0.000870644,0.00016568642,0.00040841204,0.00019316288,0.00024033929,0.0017030151],"category_scores_gemma":[0.0011502436,0.0000836394,0.00009661348,0.0005555684,0.00020355116,0.0002800996,0.00028961003,0.0001565208,0.0004476874],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007737304,0.000018694747,0.99193054,0.0000037355137,0.000010318983,0.000035691275,0.0001437629,0.000044581946,0.002066232,0.00008671869,0.00012411896,0.005458175],"study_design_scores_gemma":[4.6685642e-7,0.0000049804526,0.9996451,9.881804e-7,0.0000022634783,0.000039918148,0.00005150228,0.000064886546,0.000074115414,0.000022891385,0.0000922412,6.539839e-7],"about_ca_topic_score_codex":0.009321476,"about_ca_topic_score_gemma":0.009562231,"teacher_disagreement_score":0.009321476,"about_ca_system_score_codex":0.00023071187,"about_ca_system_score_gemma":0.0001309862,"threshold_uncertainty_score":0.018534422},"labels":[],"label_agreement":null},{"id":"W2013951064","doi":"10.1088/0004-637x/759/1/28","title":"EVIDENCE FOR A WIDE RANGE OF ULTRAVIOLET OBSCURATION IN<i>z</i>∼ 2 DUSTY GALAXIES FROM THE GOODS-<i>HERSCHEL</i>SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy; Luminous infrared galaxy; Infrared; Star formation; Astronomy; Extinction (optical mineralogy); Ultraviolet; Luminosity","score_opus":0.03855229981134458,"score_gpt":0.26469289636692345,"score_spread":0.22614059655557886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013951064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989845,0.00014675313,0.00007457456,0.000020622501,8.532168e-7,0.0000014988223,0.00018709355,0.000015221299,0.00056891784],"genre_scores_gemma":[0.99946946,0.00004674315,0.000052063857,0.000016473301,0.0000041621643,0.0000014137679,0.0003457951,0.0000028876036,0.00006104019],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996884,0.000023652285,0.00002635781,0.000089375906,0.000077965466,0.00009433642],"domain_scores_gemma":[0.9983322,0.00021616867,0.00089516275,0.00012379652,0.000113415656,0.0003192113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028925764,0.00024684778,0.0003976615,0.0020734142,0.00036601024,0.00089135044,0.0004229955,0.0003346242,0.0012730943],"category_scores_gemma":[0.00085122284,0.00027723899,0.0002467339,0.00086587004,0.0006178978,0.0004271244,0.00078171684,0.00025020156,0.0002673528],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000635937,0.000015911593,0.99003476,0.000013214075,0.000045494857,0.00008487942,0.00022073084,0.000030921,0.007512811,0.00006962788,0.00006983016,0.0018382312],"study_design_scores_gemma":[0.0000018274103,0.00001054065,0.9995229,0.000001462454,0.000005111164,0.00010946643,0.000049238435,0.00001588882,0.00018880925,0.000013866117,0.00007986198,0.0000010959482],"about_ca_topic_score_codex":0.0031518256,"about_ca_topic_score_gemma":0.005707712,"teacher_disagreement_score":0.0031518256,"about_ca_system_score_codex":0.00026975575,"about_ca_system_score_gemma":0.00010222584,"threshold_uncertainty_score":0.0062669516},"labels":[],"label_agreement":null},{"id":"W2013979799","doi":"10.1086/431923","title":"Radiation Pressure–supported Starburst Disks and Active Galactic Nucleus Fueling","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":803,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Star formation; Eddington luminosity; Radiation pressure; Luminosity; Active galactic nucleus; Opacity; Flux (metallurgy); Parsec; Galaxy; Quantum mechanics","score_opus":0.008949479387607526,"score_gpt":0.24250215521747717,"score_spread":0.23355267582986966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2013979799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9914477,0.0005590474,0.003847553,0.00015847728,0.0000137740435,0.0000072547573,0.000055637127,0.000023791494,0.0038867118],"genre_scores_gemma":[0.9991007,0.00012051705,0.0002751718,0.000010511478,0.000013199306,0.0000026716339,0.000023547525,0.0000038054588,0.00044984333],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999213,0.000018001505,0.0000047847584,0.000018790379,0.000010472375,0.000026656007],"domain_scores_gemma":[0.9996093,0.00009506915,0.00015613606,0.000039188624,0.000023881525,0.00007657415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016356465,0.0005405178,0.0004004053,0.00026061843,0.00041895,0.0013657653,0.0010518959,0.0008207682,0.0010509433],"category_scores_gemma":[0.00088357733,0.00021303416,0.00042259088,0.00020941175,0.00095944654,0.0010114147,0.00078097224,0.00032149875,0.00020691234],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003245586,0.00016808616,0.0861585,0.00014459729,0.00010650635,0.0031458847,0.00040369504,0.84156144,0.017793575,0.04379664,0.0004656269,0.005930932],"study_design_scores_gemma":[0.00011828436,0.00014813719,0.025595343,0.000022803984,0.00003763738,0.00060010207,0.00026234053,0.94836116,0.0018994139,0.021730354,0.001198032,0.000026372607],"about_ca_topic_score_codex":0.0060522156,"about_ca_topic_score_gemma":0.002213517,"teacher_disagreement_score":0.0060522156,"about_ca_system_score_codex":0.00074831746,"about_ca_system_score_gemma":0.00023473575,"threshold_uncertainty_score":0.012033999},"labels":[],"label_agreement":null},{"id":"W2014019250","doi":"10.1088/0004-637x/710/2/1557","title":"THE WEAK<i>s</i>-PROCESS IN MASSIVE STARS AND ITS DEPENDENCE ON THE NEUTRON CAPTURE CROSS SECTIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":382,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; TRIUMF","funders":"","keywords":"Nucleosynthesis; r-process; Physics; s-process; Neutron capture; Supernova; Astrophysics; Isotope; Nuclear reaction; Neutron; Nuclear physics","score_opus":0.00673995581027488,"score_gpt":0.2349135894331045,"score_spread":0.22817363362282964,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014019250","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9857349,0.00036974414,0.004641068,0.00008247896,0.000017384755,0.00001641992,0.00049544376,0.0001504361,0.008492141],"genre_scores_gemma":[0.998315,0.00013500552,0.00072044367,0.000015071896,0.0000055280148,0.000012422325,0.00022993088,0.000050459716,0.00051620044],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99988437,0.000017617389,0.000009953018,0.00003490649,0.000026512693,0.00002658754],"domain_scores_gemma":[0.99974734,0.00008503018,0.000053720873,0.00003487256,0.000035732857,0.000043258824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029536994,0.0005469859,0.00026297293,0.00038808794,0.00026122667,0.000734239,0.00049737585,0.00037786516,0.0011082159],"category_scores_gemma":[0.00091826223,0.00025902336,0.000698423,0.00038783366,0.00036758377,0.0003507568,0.00040396108,0.00021750171,0.0003452361],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039141043,0.00008390056,0.13188392,0.00017712438,0.00019691761,0.0006584529,0.00014993423,0.79373676,0.046587404,0.013282019,0.0006068449,0.01224522],"study_design_scores_gemma":[0.00009049243,0.00014054772,0.14154403,0.000034224504,0.00008950727,0.00021645984,0.000059938837,0.82894474,0.020527463,0.005606671,0.0026747268,0.00007117547],"about_ca_topic_score_codex":0.005827569,"about_ca_topic_score_gemma":0.0024332602,"teacher_disagreement_score":0.005827569,"about_ca_system_score_codex":0.00075687666,"about_ca_system_score_gemma":0.00023793455,"threshold_uncertainty_score":0.011587322},"labels":[],"label_agreement":null},{"id":"W2014131549","doi":"10.1086/345537","title":"The Cool Interstellar Medium in S0 Galaxies. I. A Survey of Molecular Gas","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Galaxy; Astrophysics; Interstellar medium; Context (archaeology); Star formation; Astronomy; Galaxy formation and evolution; Stars; Universe; Luminosity; Paleontology; Geology","score_opus":0.008090854026768185,"score_gpt":0.2134133608553008,"score_spread":0.20532250682853262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014131549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99890065,0.00040823073,0.00003289679,0.000020321511,7.8890616e-7,0.0000019115132,0.00025931458,0.00000677176,0.0003690684],"genre_scores_gemma":[0.99883634,0.0002961828,0.00007759797,0.000024563706,0.0000057634225,0.0000026873888,0.00048342912,0.000001579271,0.0002717903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992085,0.000010512575,0.000004688132,0.000022122886,0.000016849637,0.000025083938],"domain_scores_gemma":[0.99964046,0.000037937796,0.00016109906,0.000017076014,0.0000284848,0.00011496213],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001433968,0.00018334018,0.00015518333,0.001868352,0.0002851349,0.00056269136,0.00022193824,0.000214238,0.0012246],"category_scores_gemma":[0.0003164677,0.00010425726,0.00012646975,0.0012391147,0.00043786608,0.000465208,0.000508582,0.00010139741,0.00037148158],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059384958,0.00002162242,0.9885765,0.000022886448,0.000017088681,0.00007711414,0.00039906322,0.00003257135,0.0057165516,0.00012638261,0.00017225019,0.0047786124],"study_design_scores_gemma":[0.0000010206259,0.000024548155,0.99914503,0.000002822105,0.0000052533637,0.000092219765,0.00017660079,0.000036339898,0.00017508301,0.000025732576,0.00031428738,9.2640494e-7],"about_ca_topic_score_codex":0.006534818,"about_ca_topic_score_gemma":0.01262127,"teacher_disagreement_score":0.006534818,"about_ca_system_score_codex":0.00024563866,"about_ca_system_score_gemma":0.00010046748,"threshold_uncertainty_score":0.012993574},"labels":[],"label_agreement":null},{"id":"W2014203674","doi":"10.1088/0004-637x/736/2/89","title":"HIGH-CONTRAST IMAGING SEARCH FOR PLANETS AND BROWN DWARFS AROUND THE MOST MASSIVE STARS IN THE SOLAR NEIGHBORHOOD","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Physics; Planet; Astrophysics; Stars; Brown dwarf; Astronomy; Instability; Population; Planetary system; Accretion (finance); Planetary mass; Exoplanet","score_opus":0.01579927408345385,"score_gpt":0.2240636584648925,"score_spread":0.20826438438143866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014203674","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962954,0.00018008258,0.0014313693,0.00003916919,0.0000026458965,0.000010169258,0.00016778549,0.00005626438,0.0018171184],"genre_scores_gemma":[0.9962769,0.00006366673,0.0030919248,0.000027450049,0.000011477309,0.0000035925473,0.00020416202,0.000005951715,0.00031468322],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999416,0.000006525382,0.0000031914526,0.000019314368,0.000012975713,0.000016331007],"domain_scores_gemma":[0.9997774,0.00003644726,0.000049503793,0.000018817764,0.000040087405,0.000077811506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017363865,0.000120813114,0.00012700839,0.0008956809,0.00027082546,0.00030918967,0.00017117153,0.0002814367,0.0013422864],"category_scores_gemma":[0.00033172898,0.00012952172,0.00010075155,0.0002779125,0.00010703801,0.0002511789,0.00029480137,0.00012683049,0.0002637463],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016612212,0.00013064829,0.70652294,0.00010335642,0.00008631619,0.0010001492,0.0005104668,0.00053161,0.26314235,0.0003473247,0.0011676331,0.026290944],"study_design_scores_gemma":[0.0000057644247,0.00009373245,0.98383796,0.000009764211,0.00003175087,0.0016808958,0.00025026113,0.0013453676,0.011332677,0.00012652235,0.0012802444,0.000005012065],"about_ca_topic_score_codex":0.0008121325,"about_ca_topic_score_gemma":0.0027133913,"teacher_disagreement_score":0.0013422864,"about_ca_system_score_codex":0.00009568617,"about_ca_system_score_gemma":0.00006684835,"threshold_uncertainty_score":0.004490435},"labels":[],"label_agreement":null},{"id":"W2014234601","doi":"10.1086/323771","title":"Globular Cluster Population of Hickson Compact Group 22a and 90c","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Galaxy; Galaxy cluster; Astronomy; Population; Cluster (spacecraft); Medicine; Computer science","score_opus":0.007284929418224178,"score_gpt":0.21701870038819535,"score_spread":0.20973377096997117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014234601","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983747,0.000067290224,0.000059242455,0.000008778245,0.0000015960019,0.000007933933,0.0002172064,0.0000067205597,0.0012565679],"genre_scores_gemma":[0.9985164,0.000032150663,0.000107276144,0.00002217426,0.0000062383697,0.0000069498005,0.00088240055,0.00000570312,0.00042083746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962366,0.000028519766,0.000018528915,0.00012420054,0.00010548939,0.000099682555],"domain_scores_gemma":[0.99929225,0.000044591827,0.00019045967,0.000060341077,0.000100725825,0.0003115635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037104485,0.00030351806,0.00025827665,0.0015590444,0.00043953987,0.00070006703,0.0003728534,0.00025116932,0.0013252856],"category_scores_gemma":[0.0008038909,0.00013832806,0.00012279314,0.0007247239,0.00049174996,0.0003425567,0.00095084595,0.0001948319,0.0005278068],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018701558,0.000048661772,0.9832819,0.00001166124,0.000027136632,0.00014536813,0.0005680685,0.000071141425,0.009231705,0.000284706,0.00035069138,0.0057919426],"study_design_scores_gemma":[0.000006149761,0.00007675168,0.99812824,0.0000029056696,0.0000074707687,0.0002738876,0.00016016164,0.00007368584,0.0004818103,0.000039250677,0.00074487255,0.0000048527436],"about_ca_topic_score_codex":0.010864317,"about_ca_topic_score_gemma":0.009429584,"teacher_disagreement_score":0.010864317,"about_ca_system_score_codex":0.00050162757,"about_ca_system_score_gemma":0.00016115318,"threshold_uncertainty_score":0.021602154},"labels":[],"label_agreement":null},{"id":"W2014246403","doi":"10.1088/0004-637x/774/1/7","title":"SIMPLE ANALYTICAL FORMS OF THE PERPENDICULAR DIFFUSION COEFFICIENT FOR TWO-COMPONENT TURBULENCE. I. MAGNETOSTATIC TURBULENCE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Perpendicular; Diffusion; Turbulence; Computational physics; Magnetic field; Classical mechanics; Mechanics; Geometry; Quantum mechanics","score_opus":0.005651871039997274,"score_gpt":0.22810195608388578,"score_spread":0.2224500850438885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014246403","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.122194804,0.0037590025,0.8136507,0.0010744747,0.00049600995,0.00031850176,0.00058136566,0.00081988005,0.057105195],"genre_scores_gemma":[0.9069677,0.0033085763,0.072013736,0.0002680141,0.00020096543,0.00024265343,0.00037279938,0.0003290508,0.016296482],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998497,0.000025988329,0.000012869647,0.000031219206,0.000054439624,0.000025770845],"domain_scores_gemma":[0.9994118,0.00021897296,0.00012902882,0.00006395197,0.00013494071,0.00004131003],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039160962,0.0011365787,0.0004804204,0.0009850665,0.00047659036,0.0012589392,0.0007076174,0.0009432134,0.0030691454],"category_scores_gemma":[0.0032714661,0.0002747225,0.0005233206,0.0006108778,0.00091288635,0.002044888,0.0007085071,0.0009575106,0.0006600092],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060128477,0.000105721156,0.0011034347,0.00046429312,0.000028519884,0.00051486434,0.0002926469,0.10890365,0.06751449,0.7959443,0.004978004,0.020090017],"study_design_scores_gemma":[0.000023802651,0.000029416746,0.0008178636,0.00006434579,0.000016438786,0.00060184137,0.000069534384,0.8112581,0.0061599943,0.17541088,0.005452193,0.00009561352],"about_ca_topic_score_codex":0.0012291184,"about_ca_topic_score_gemma":0.0010204708,"teacher_disagreement_score":0.0030691454,"about_ca_system_score_codex":0.0007563882,"about_ca_system_score_gemma":0.0005444003,"threshold_uncertainty_score":0.010267258},"labels":[],"label_agreement":null},{"id":"W2014449273","doi":"10.1088/0004-637x/711/2/1157","title":"DYNAMICAL INFERENCE FROM A KINEMATIC SNAPSHOT: THE FORCE LAW IN THE SOLAR SYSTEM","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Kinematics; Population; Solar System; Inference; Gravitation; Gravitational acceleration; Snapshot (computer storage); Dynamical systems theory; Frequentist inference","score_opus":0.009332846378922942,"score_gpt":0.2647271308203632,"score_spread":0.25539428444144024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014449273","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.24699335,0.00073910464,0.7480446,0.0007218377,0.00005548195,0.000025403666,0.00074171054,0.00051667396,0.0021617597],"genre_scores_gemma":[0.91498786,0.00033678644,0.083132505,0.00012764771,0.00009132981,0.000016486914,0.0007206427,0.00006588398,0.0005208876],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9993938,0.00019825301,0.000029312763,0.00023773304,0.00010661382,0.000034226654],"domain_scores_gemma":[0.9951224,0.0034376436,0.00057022495,0.00056877645,0.000186452,0.00011446917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023004834,0.0003733186,0.00056053576,0.000998655,0.00060014444,0.0012668847,0.00106056,0.00066757173,0.00097311346],"category_scores_gemma":[0.019445797,0.00046279677,0.00068564975,0.00084339385,0.0010662256,0.002284561,0.0010793945,0.0015311299,0.00015805477],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004721924,0.00012865913,0.24284005,0.00030047382,0.00088427606,0.0010804738,0.0013896564,0.38676268,0.014560337,0.17846817,0.0033009076,0.16981217],"study_design_scores_gemma":[0.000050043767,0.00003857583,0.055031415,0.00006284195,0.00014338183,0.00035700484,0.00016054572,0.8218273,0.0039462885,0.11539201,0.0029129481,0.00007771714],"about_ca_topic_score_codex":0.013816984,"about_ca_topic_score_gemma":0.012220346,"teacher_disagreement_score":0.013816984,"about_ca_system_score_codex":0.00071466423,"about_ca_system_score_gemma":0.0006242388,"threshold_uncertainty_score":0.027473092},"labels":[],"label_agreement":null},{"id":"W2014555677","doi":"10.1088/0004-637x/777/1/5","title":"THE CO-TO-H<sub>2</sub>CONVERSION FACTOR AND DUST-TO-GAS RATIO ON KILOPARSEC SCALES IN NEARBY GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":600,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Astrophysics; Physics; Environmental science; Materials science","score_opus":0.009052575704244207,"score_gpt":0.22518178309087275,"score_spread":0.21612920738662855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014555677","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975138,0.00012870519,0.00030256438,0.000028613467,0.0000019347965,0.0000015985144,0.00071763364,0.000048966976,0.0012562916],"genre_scores_gemma":[0.99858814,0.000045254834,0.00035112372,0.0000102530275,0.0000042032298,0.0000029351668,0.0006818782,0.000015510856,0.00030071518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992335,0.000008840265,0.000004380825,0.000037140435,0.000012046862,0.000014262846],"domain_scores_gemma":[0.9996239,0.00011281876,0.000113362876,0.000044358792,0.000044569882,0.000061004688],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013066211,0.00014833154,0.00013432879,0.00091981434,0.00014706979,0.0004014131,0.00024655188,0.00023376953,0.0015484478],"category_scores_gemma":[0.00049584213,0.00021129222,0.00023280556,0.0007224387,0.00023915955,0.00026455775,0.00022298138,0.00023764366,0.00036565572],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033426227,0.000045593755,0.93885446,0.00004762362,0.00015930245,0.00019568858,0.00022697805,0.0062980168,0.039201804,0.00071900716,0.00097336504,0.0129438825],"study_design_scores_gemma":[0.0000015719656,0.0000047555977,0.9979644,0.0000013611742,0.0000081931175,0.000038672824,0.000046250094,0.0009964121,0.0007190727,0.000059050162,0.00015719717,0.0000031350316],"about_ca_topic_score_codex":0.014651961,"about_ca_topic_score_gemma":0.015097353,"teacher_disagreement_score":0.014651961,"about_ca_system_score_codex":0.00030215012,"about_ca_system_score_gemma":0.00006142309,"threshold_uncertainty_score":0.02913332},"labels":[],"label_agreement":null},{"id":"W2014590217","doi":"10.1086/425980","title":"Continuum Acceleration of Black Hole Winds","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Black-body radiation; Ionization; Launched; Plasma; Spectral line; Absorption (acoustics)","score_opus":0.014813275116622905,"score_gpt":0.23786706161346488,"score_spread":0.223053786496842,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014590217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96358556,0.00032940475,0.0171087,0.00011161722,0.000039439667,0.000030335628,0.00008680861,0.00017126797,0.018536841],"genre_scores_gemma":[0.9968252,0.00012147805,0.00085862185,0.000017724113,0.00001776393,0.0000070756123,0.00005091133,0.000010513895,0.0020908103],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995065,0.000008701198,0.0000018096731,0.000009577436,0.000011234947,0.000018118326],"domain_scores_gemma":[0.9998934,0.000017441847,0.000031278087,0.000012367604,0.000013642171,0.000031976797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008843969,0.00041788167,0.0001813631,0.00019539018,0.00027657027,0.00058769394,0.00035567116,0.0003737404,0.0020568224],"category_scores_gemma":[0.0002967734,0.00015503129,0.00048411064,0.00009040332,0.0003356468,0.00043477572,0.00053124427,0.00025869612,0.00029382407],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009253078,0.0002872907,0.15835884,0.0001974278,0.00016222283,0.004775496,0.0007597472,0.5085677,0.14601511,0.14600061,0.0022599811,0.03169029],"study_design_scores_gemma":[0.00026864378,0.00057743664,0.101266205,0.00003828055,0.00005766447,0.0012555091,0.00018101318,0.8492281,0.008974106,0.033037577,0.0050431346,0.00007239198],"about_ca_topic_score_codex":0.0021035532,"about_ca_topic_score_gemma":0.0011909412,"teacher_disagreement_score":0.0021035532,"about_ca_system_score_codex":0.0004294917,"about_ca_system_score_gemma":0.00014687318,"threshold_uncertainty_score":0.00688082},"labels":[],"label_agreement":null},{"id":"W2014620781","doi":"10.1088/0004-637x/707/2/921","title":"IRAS 16293: A “MAGNETIC” TALE OF TWO CORES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Physics; Astrophysics; Magnetic field; Polarization (electrochemistry); Submillimeter Array; Star formation; Perpendicular; Geometry; Stars","score_opus":0.008750332499038177,"score_gpt":0.24997003559675615,"score_spread":0.24121970309771798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014620781","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99582064,0.0000973542,0.0004785149,0.000064773565,0.00001055763,0.0000066029224,0.0001803762,0.00006546938,0.0032756585],"genre_scores_gemma":[0.9981925,0.000020938776,0.0010432715,0.000043454726,0.00001709909,0.0000026724144,0.00040042048,0.000009799386,0.00026988846],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999471,0.0000054779002,0.000002394001,0.000016052396,0.000014760249,0.000014235367],"domain_scores_gemma":[0.99984574,0.000009841111,0.00005844954,0.000014216383,0.000016027949,0.00005583281],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010330732,0.0001352716,0.00012001226,0.00059504516,0.00039459518,0.00037828452,0.00025645888,0.0002944101,0.0010186015],"category_scores_gemma":[0.0002849977,0.00013147497,0.0000838887,0.0005376583,0.00021248947,0.00026063732,0.00034321786,0.00022577275,0.00029461255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016357261,0.0006613969,0.5595464,0.00021974374,0.0001308381,0.004619556,0.0015290013,0.0020397622,0.3520842,0.0054696673,0.008783075,0.063280635],"study_design_scores_gemma":[0.0000826187,0.00025681965,0.97309846,0.0000273088,0.000041166964,0.002169408,0.00036969478,0.005220946,0.008603589,0.0015291963,0.008579495,0.000021343294],"about_ca_topic_score_codex":0.0013259314,"about_ca_topic_score_gemma":0.0025844725,"teacher_disagreement_score":0.0013259314,"about_ca_system_score_codex":0.00017026921,"about_ca_system_score_gemma":0.000078606594,"threshold_uncertainty_score":0.0034075975},"labels":[],"label_agreement":null},{"id":"W2014727289","doi":"10.1088/0004-637x/734/1/52","title":"EFFECTS OF STRONG GRAVITATIONAL LENSING ON MILLIMETER-WAVE GALAXY NUMBER COUNTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Gravitational lens; Halo; Source counts; Redshift; Millimeter; Flux (metallurgy); Weak gravitational lensing; Lens (geology); Astronomy; Optics","score_opus":0.014657185549824245,"score_gpt":0.21916348468439653,"score_spread":0.2045062991345723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014727289","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9916687,0.00014744794,0.0060462067,0.00009035275,0.0000053417048,0.000011232389,0.00014374085,0.00010144168,0.0017855278],"genre_scores_gemma":[0.9990133,0.00005197666,0.00071565754,0.000012142796,0.000004143587,0.0000036298518,0.000063399966,0.000012857533,0.0001228397],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99943537,0.00023168346,0.00003107195,0.00009308655,0.000115340874,0.00009346514],"domain_scores_gemma":[0.9887638,0.0077376673,0.0018578966,0.0006651715,0.00049291016,0.00048256852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015923559,0.000862937,0.00045861857,0.0005727731,0.00035452438,0.000932151,0.0006392718,0.00049842586,0.001122769],"category_scores_gemma":[0.011682777,0.00045149628,0.0007333509,0.00051634415,0.00075425365,0.0009944717,0.00095792394,0.00046487656,0.00015762914],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027372868,0.000046182293,0.11366831,0.00006168556,0.00009460839,0.00031153567,0.00006672491,0.8720624,0.0047445316,0.004062277,0.00016977765,0.004438215],"study_design_scores_gemma":[0.00005716656,0.00024613857,0.05379453,0.000014901826,0.00005584704,0.00014891392,0.000045445428,0.9356796,0.0072255316,0.0024610562,0.0002331427,0.000037787202],"about_ca_topic_score_codex":0.004469231,"about_ca_topic_score_gemma":0.0039965734,"teacher_disagreement_score":0.004469231,"about_ca_system_score_codex":0.0012321819,"about_ca_system_score_gemma":0.00036440295,"threshold_uncertainty_score":0.008940101},"labels":[],"label_agreement":null},{"id":"W2014763623","doi":"10.1088/0004-637x/743/2/167","title":"STRUCTURE AND DYNAMICS OF THE GLOBULAR CLUSTER PALOMAR 13","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Velocity dispersion; Metallicity; Photometry (optics); Star cluster; Stellar dynamics; Luminosity; Mass segregation; Radial velocity","score_opus":0.0070874116673299336,"score_gpt":0.19101592508017035,"score_spread":0.18392851341284042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014763623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99558455,0.00007342582,0.00016437373,0.00005772868,0.0000023183356,0.000006390443,0.00024371066,0.00003262775,0.0038348236],"genre_scores_gemma":[0.99718094,0.000053347554,0.0004523373,0.000020642181,0.0000035074859,0.000008480191,0.00095688965,0.0000125527795,0.0013113108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990785,0.0000058742503,0.0000030175997,0.000033838714,0.000026721696,0.000022761176],"domain_scores_gemma":[0.9996861,0.000020377794,0.000060803795,0.000016626733,0.00010356636,0.000112580936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012595166,0.00017070245,0.00016358725,0.00086496543,0.0006702681,0.00063115836,0.00045306367,0.00016717258,0.0021611175],"category_scores_gemma":[0.0004149256,0.00012792191,0.00015143909,0.0008718104,0.0004723141,0.00020451607,0.00088792207,0.00023379631,0.0005327584],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012906843,0.000054039243,0.96414244,0.000030373083,0.000031503587,0.00048094447,0.0014481249,0.0028651375,0.01000545,0.0020306949,0.0022695318,0.016512694],"study_design_scores_gemma":[0.00000678297,0.000036218662,0.99136764,0.000008597241,0.000007705091,0.00015853855,0.0004131088,0.0037568668,0.0004913125,0.0004220176,0.0033203578,0.000010727106],"about_ca_topic_score_codex":0.0359713,"about_ca_topic_score_gemma":0.037356388,"teacher_disagreement_score":0.0359713,"about_ca_system_score_codex":0.001369002,"about_ca_system_score_gemma":0.00045079723,"threshold_uncertainty_score":0.071523845},"labels":[],"label_agreement":null},{"id":"W2014778256","doi":"10.1086/513510","title":"First Detection of Phase-dependent Colliding Wind X-Ray Emission outside the Milky Way","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Hôpital Notre-Dame","funders":"","keywords":"Milky Way; Ejecta; Physics; Astrophysics; X-ray; Astronomy; Binary number; Galaxy; Optics; Supernova","score_opus":0.0133695205710307,"score_gpt":0.24533363797010246,"score_spread":0.23196411739907177,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014778256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988482,0.0001246132,0.00021191279,0.000015385425,0.000004848081,0.000004836315,0.000027450329,0.000009778536,0.00075305847],"genre_scores_gemma":[0.9991555,0.000046342582,0.0003212953,0.00001527224,0.000010585311,0.0000031410311,0.00008507651,0.000006059602,0.0003566506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998927,0.000011739279,0.0000052848022,0.000029928226,0.000028294238,0.000032146105],"domain_scores_gemma":[0.9996178,0.00006225429,0.00012490037,0.000052096373,0.000057017958,0.00008592894],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001345049,0.00013127216,0.00022404222,0.0004805995,0.0004521018,0.0005592843,0.00026967577,0.0004157949,0.0006808953],"category_scores_gemma":[0.0004991079,0.00019562413,0.00016263743,0.00023317765,0.0003042708,0.00024444293,0.00076498126,0.00032713925,0.00018343689],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004894824,0.00014807792,0.68712807,0.00012324443,0.0001370231,0.0090924725,0.0018393582,0.00020708962,0.27901638,0.00082632515,0.00046607672,0.020526387],"study_design_scores_gemma":[0.000014498031,0.00030998923,0.9861268,0.000012708553,0.000025216985,0.0028848415,0.0002441385,0.00026846275,0.0076611657,0.00013094788,0.0023129974,0.000008283291],"about_ca_topic_score_codex":0.0005536252,"about_ca_topic_score_gemma":0.0015204505,"teacher_disagreement_score":0.0006808953,"about_ca_system_score_codex":0.00016052256,"about_ca_system_score_gemma":0.00013408679,"threshold_uncertainty_score":0.0022777915},"labels":[],"label_agreement":null},{"id":"W2014824950","doi":"10.1086/508986","title":"The ACS Virgo Cluster Survey. XIV. Analysis of Color‐Magnitude Relations in Globular Cluster Systems","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Cluster (spacecraft); Virgo Cluster; Galaxy cluster; Star cluster; Blue straggler; Galaxy groups and clusters","score_opus":0.006534751786443236,"score_gpt":0.21449885186904913,"score_spread":0.20796410008260588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014824950","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.13371173,0.0017998803,0.0014728295,0.0034640906,0.0010824766,0.0005320999,0.79312736,0.0046230815,0.06018652],"genre_scores_gemma":[0.25860226,0.0010320183,0.003868414,0.00052689534,0.00074848975,0.00034184993,0.6520928,0.0014552723,0.08133195],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99952185,0.000057639605,0.00003166744,0.00006628036,0.00022355228,0.00009905749],"domain_scores_gemma":[0.9957885,0.00042168834,0.0004630579,0.0006878417,0.00183865,0.000800209],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011238379,0.00040906158,0.0005267062,0.0061145313,0.0006134564,0.00094127696,0.0009746445,0.00039736874,0.041746367],"category_scores_gemma":[0.004766431,0.00043832356,0.00037585455,0.0047811996,0.0002005845,0.0005161692,0.0010068523,0.0004318029,0.029309593],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002095823,0.000093165276,0.11712603,0.0003010712,0.00008940438,0.00014299974,0.000116758405,0.0002309461,0.0014119924,0.00048336945,0.806453,0.073341675],"study_design_scores_gemma":[0.00010379753,0.00004475069,0.8055794,0.000053258635,0.000061430124,0.000078824,0.00014391645,0.00039895973,0.0009805807,0.00040117968,0.19212644,0.000027430315],"about_ca_topic_score_codex":0.030393029,"about_ca_topic_score_gemma":0.049379174,"teacher_disagreement_score":0.041746367,"about_ca_system_score_codex":0.00038197823,"about_ca_system_score_gemma":0.00092310936,"threshold_uncertainty_score":0.13965553},"labels":[],"label_agreement":null},{"id":"W2014932747","doi":"10.1086/509313","title":"The Central Engines of Narrow‐Line Seyfert 1 Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University; York University","funders":"","keywords":"Astrophysics; Physics; Bulge; Galaxy; Black hole (networking); Astronomy; Luminosity; Solar mass; Virial theorem; Supermassive black hole; Active galactic nucleus; Line (geometry); Geometry","score_opus":0.006204355588478551,"score_gpt":0.21136965806832061,"score_spread":0.20516530247984208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2014932747","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99641305,0.00039003775,0.0003375109,0.00005152111,0.000005436337,0.000007741307,0.00022084134,0.000056627676,0.0025171782],"genre_scores_gemma":[0.9971724,0.00020922138,0.0005366262,0.000019678151,0.000011788591,0.000007875875,0.0005284991,0.000005588348,0.0015084194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999496,0.000002371592,0.0000026490295,0.000015566464,0.00001078018,0.000019077961],"domain_scores_gemma":[0.9997646,0.000027847203,0.00011367884,0.00002210256,0.000022165825,0.000049622082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014462719,0.00027650117,0.00022325879,0.0008006957,0.0003910329,0.00091005914,0.00027524657,0.00026380512,0.004280153],"category_scores_gemma":[0.0004346964,0.00017319649,0.00018126403,0.00043240326,0.00025996153,0.00047297386,0.00043691753,0.00017108717,0.00077696604],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005599321,0.00014554267,0.8119651,0.00020440925,0.00009044951,0.0014366437,0.0015080569,0.0037479536,0.08994334,0.007024525,0.004112045,0.0792619],"study_design_scores_gemma":[0.00003642645,0.00013150433,0.9810543,0.000034913304,0.000033294564,0.0007334674,0.00043577855,0.0038909647,0.004593064,0.0017025719,0.007337375,0.000016311807],"about_ca_topic_score_codex":0.004146852,"about_ca_topic_score_gemma":0.0042072814,"teacher_disagreement_score":0.004280153,"about_ca_system_score_codex":0.00033742184,"about_ca_system_score_gemma":0.00018507038,"threshold_uncertainty_score":0.014318526},"labels":[],"label_agreement":null},{"id":"W2015011554","doi":"10.1086/427776","title":"PSR J1756-2251: A New Relativistic Double Neutron Star System","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":149,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Pulsar; Neutron star; Binary pulsar; Astrophysics; Gravitational wave; Eccentricity (behavior); Orbital period; Astronomy; Orbital elements; General relativity; Gravitational redshift; Millisecond pulsar; Stars; Classical mechanics","score_opus":0.015374582031104327,"score_gpt":0.29959099877071993,"score_spread":0.2842164167396156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015011554","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963613,0.0007982174,0.00036773874,0.00014767311,0.000038605656,0.000016649228,0.00012738282,0.000057045505,0.0020853288],"genre_scores_gemma":[0.9978047,0.00023061736,0.0007568401,0.00010965691,0.00005002026,0.000006609122,0.00043206647,0.000006240371,0.000603237],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998691,0.000010628329,0.000011838386,0.000042160715,0.00003325053,0.00003298108],"domain_scores_gemma":[0.99978334,0.0000104703395,0.000089951005,0.000021425632,0.000015334246,0.00007944313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021065817,0.00040176167,0.00041855025,0.00071344344,0.0009864363,0.00077198696,0.00049785327,0.00040267655,0.0011164901],"category_scores_gemma":[0.00036194135,0.0001780284,0.00015734442,0.0005144111,0.0004195617,0.00030650216,0.0009705639,0.00041992322,0.00056399003],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011511146,0.0003836008,0.71301454,0.00036926428,0.00021634827,0.03881666,0.0020091904,0.0013770063,0.13096067,0.005823029,0.0057031857,0.100175425],"study_design_scores_gemma":[0.00017991278,0.0013181801,0.85777885,0.000039635506,0.00019397635,0.08335342,0.00063267065,0.0021729968,0.009957194,0.0021875266,0.04210169,0.000083935425],"about_ca_topic_score_codex":0.0015688862,"about_ca_topic_score_gemma":0.0029443481,"teacher_disagreement_score":0.0015688862,"about_ca_system_score_codex":0.00046023392,"about_ca_system_score_gemma":0.00024444808,"threshold_uncertainty_score":0.0037350059},"labels":[],"label_agreement":null},{"id":"W2015058398","doi":"10.1088/0004-637x/726/2/113","title":"TWO WIDE PLANETARY-MASS COMPANIONS TO SOLAR-TYPE STARS IN UPPER SCORPIUS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":168,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Brown dwarf; Stars; Binary number; Planet; Binary star; Circumbinary planet; Primary (astronomy); Solar mass","score_opus":0.010435221651905587,"score_gpt":0.23728373259843563,"score_spread":0.22684851094653005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015058398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99840015,0.000037095397,0.000057367903,0.00001486462,0.0000010041568,0.0000037980171,0.00007651728,0.000012478993,0.0013968023],"genre_scores_gemma":[0.9984939,0.000060707775,0.00021019088,0.000017283903,0.0000033523568,0.0000048412617,0.00033096469,0.000004891868,0.00087396434],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988544,0.0000045353418,0.0000053707104,0.000038960367,0.00002783445,0.000037843733],"domain_scores_gemma":[0.99971205,0.000029814832,0.00010198408,0.000021731415,0.000033016804,0.00010133151],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008549451,0.0001840234,0.0001550335,0.00142806,0.0007531023,0.00051862077,0.00020087331,0.00023477178,0.0013268983],"category_scores_gemma":[0.0002527288,0.00016035182,0.00010521665,0.0006169125,0.00057541655,0.00031261344,0.0009796647,0.00021837966,0.00026441098],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005968181,0.000050608756,0.95112234,0.0000312094,0.00001401028,0.0014205148,0.0022078482,0.0001342554,0.018305354,0.00016975406,0.00044966774,0.026034666],"study_design_scores_gemma":[9.793144e-7,0.000015664327,0.99822634,0.000006408115,0.000003484281,0.0003529135,0.00047512513,0.00006579304,0.00030015048,0.000024930081,0.00052620453,0.000001953472],"about_ca_topic_score_codex":0.026822533,"about_ca_topic_score_gemma":0.07741633,"teacher_disagreement_score":0.026822533,"about_ca_system_score_codex":0.000388021,"about_ca_system_score_gemma":0.0003402047,"threshold_uncertainty_score":0.053332806},"labels":[],"label_agreement":null},{"id":"W2015135734","doi":"10.1086/428116","title":"Asteroseismology of the Crystallized ZZ Ceti Star BPM 37093: A Different View","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Asteroseismology; Physics; White dwarf; Astrophysics; Value (mathematics); Core (optical fiber); Fraction (chemistry); Stars; Theoretical physics; Statistics; Mathematics; Optics","score_opus":0.011393220738459085,"score_gpt":0.223024158046125,"score_spread":0.2116309373076659,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015135734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9582358,0.0021495353,0.01620521,0.0024867,0.000080825375,0.000015957667,0.0011770269,0.00040750438,0.019241327],"genre_scores_gemma":[0.9947537,0.0005619642,0.003084343,0.00019087113,0.00007801836,0.0000045088736,0.0006279857,0.000081873186,0.00061663246],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998641,0.000016753058,0.0000085161155,0.00005188235,0.000039306156,0.000019489642],"domain_scores_gemma":[0.9995814,0.00006628039,0.000082372426,0.00013484497,0.000054537664,0.000080616664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004357496,0.00029932937,0.00053404144,0.0007723498,0.00041876273,0.0016209208,0.0005123143,0.0005468696,0.0012902232],"category_scores_gemma":[0.0011458937,0.00013841751,0.00047874014,0.0005372075,0.0008594565,0.0014133273,0.0008095576,0.00082431996,0.00023104712],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019031815,0.00019551703,0.4960551,0.00088557875,0.0006109319,0.001924916,0.0044756113,0.06594442,0.19930023,0.110028595,0.004972936,0.11370307],"study_design_scores_gemma":[0.000104025734,0.00027650723,0.7116722,0.00018813935,0.00021093848,0.0017774216,0.0023865802,0.13316971,0.026347468,0.091612086,0.032093056,0.0001618721],"about_ca_topic_score_codex":0.002831703,"about_ca_topic_score_gemma":0.0012379363,"teacher_disagreement_score":0.002831703,"about_ca_system_score_codex":0.000658688,"about_ca_system_score_gemma":0.00035933268,"threshold_uncertainty_score":0.0056304336},"labels":[],"label_agreement":null},{"id":"W2015212959","doi":"10.1086/317773","title":"Excitation Analysis of SO and SO<sub>2</sub>in the Proto–Planetary Nebula OH 231.8+4.2","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Envelope (radar); Planetary nebula; Nebula; Astrophysics; Bipolar outflow; Excitation; Rotation (mathematics); Outflow; Atomic physics; Emission spectrum; Bipolar nebula; Millimeter; Stars; Astronomy; Spectral line; Emission nebula; Star formation; Geometry","score_opus":0.006960674343583818,"score_gpt":0.22341750925292994,"score_spread":0.2164568349093461,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015212959","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993767,0.000040154773,0.00011038673,0.000004825754,5.1833763e-7,0.0000012650663,0.000055219767,0.0000059255017,0.0004050344],"genre_scores_gemma":[0.9993488,0.000028896035,0.00013596339,0.0000056218105,0.0000012157786,0.0000018344181,0.00021357104,0.000003930342,0.0002602333],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996495,0.0000024059593,0.0000012932842,0.000011384587,0.000007922826,0.000012034823],"domain_scores_gemma":[0.99995434,0.000009807718,0.000012731796,0.0000038383664,0.000008645084,0.000010604368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004994529,0.00016173876,0.00012609574,0.0003698085,0.00017379702,0.0002472852,0.000098842145,0.00013778241,0.0010884892],"category_scores_gemma":[0.00013151234,0.00010929139,0.00011383654,0.00016800464,0.0001025671,0.00012020018,0.00016436607,0.000113046764,0.00018855765],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004985412,0.00003833495,0.15333809,0.00004945729,0.00004392773,0.0003456456,0.00017537193,0.0021103446,0.8332793,0.00047073717,0.00011236075,0.009537808],"study_design_scores_gemma":[0.000014888673,0.00008437405,0.9272725,0.000005133154,0.000022372062,0.0002241128,0.00012510555,0.007102318,0.063841134,0.00024915187,0.0010445701,0.000014275239],"about_ca_topic_score_codex":0.0021449898,"about_ca_topic_score_gemma":0.0035653522,"teacher_disagreement_score":0.0021449898,"about_ca_system_score_codex":0.00023532599,"about_ca_system_score_gemma":0.00008422881,"threshold_uncertainty_score":0.0042650104},"labels":[],"label_agreement":null},{"id":"W2015241906","doi":"10.1086/308355","title":"<i>Infrared Space Observatory</i>Spectroscopy of Extreme Carbon Stars","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Stars; Carbon star; Infrared; Astronomy; Spectral line; Line (geometry); Cosmic dust; Planetary nebula; Interstellar medium; Circumstellar dust; Astronomical spectroscopy; Space observatory; Feature (linguistics); Carbon fibers; Galaxy","score_opus":0.014934146231409071,"score_gpt":0.2282777748969754,"score_spread":0.21334362866556633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015241906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99797434,0.000105817606,0.00025964298,0.000023190818,0.00000354243,0.000003910018,0.00042123182,0.000039111655,0.0011691682],"genre_scores_gemma":[0.9970361,0.000075752025,0.0010703624,0.000024030076,0.000010680665,0.0000051346874,0.0014919036,0.000005305466,0.00028076637],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999254,0.0000070975902,0.000004493546,0.000019183864,0.000024954657,0.000018858476],"domain_scores_gemma":[0.9997489,0.00003167445,0.000102941645,0.000018413364,0.0000340556,0.0000640231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019633534,0.00035536409,0.0001117155,0.0010570977,0.00032895256,0.00034394683,0.00030301992,0.00029414918,0.00090734434],"category_scores_gemma":[0.00023245311,0.0001132859,0.00019341592,0.0006946076,0.00013533121,0.00017913981,0.00024672918,0.0001641025,0.00015555475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019373774,0.00010861786,0.9498083,0.000055067903,0.000091484166,0.00039334115,0.00009677261,0.003586708,0.031981338,0.00032649783,0.0011365119,0.012221562],"study_design_scores_gemma":[0.000011633846,0.00007788254,0.9905042,0.0000063540147,0.000025300486,0.00023388717,0.000039156348,0.004773007,0.003116746,0.00011546068,0.001090384,0.0000059830923],"about_ca_topic_score_codex":0.003938601,"about_ca_topic_score_gemma":0.008184657,"teacher_disagreement_score":0.003938601,"about_ca_system_score_codex":0.00030553006,"about_ca_system_score_gemma":0.00011608482,"threshold_uncertainty_score":0.007831395},"labels":[],"label_agreement":null},{"id":"W2015305364","doi":"10.1088/0004-637x/721/1/26","title":"PRECISE BLACK HOLE MASSES FROM MEGAMASER DISKS: BLACK HOLE-BULGE RELATIONS AT LOW MASS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":257,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Bulge; Galaxy; Velocity dispersion; Megamaser; Elliptical galaxy; Stellar mass; Black hole (networking); Astronomy; Galaxy rotation curve; Stellar kinematics; Galaxy formation and evolution; Star formation; Milky Way","score_opus":0.0069701180659231836,"score_gpt":0.21324211488280242,"score_spread":0.20627199681687924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015305364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983177,0.00019352429,0.000625877,0.000012180254,0.0000010658589,0.0000024909773,0.00019821317,0.00001915927,0.00062981143],"genre_scores_gemma":[0.99936575,0.00003688886,0.00031680334,0.000004784878,0.0000027268122,0.0000011883648,0.00019210587,0.0000026709665,0.00007704359],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999119,0.000010113698,0.0000047996764,0.00002929109,0.000020225283,0.000023633353],"domain_scores_gemma":[0.9995616,0.00009054568,0.00018352726,0.000058631205,0.000034295037,0.000071388786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020884744,0.00023436474,0.000231701,0.0010039451,0.0002749405,0.000626258,0.00023289614,0.00021881257,0.0013179397],"category_scores_gemma":[0.00073821994,0.000110019995,0.00012947875,0.00055241416,0.00024829162,0.0004472353,0.0005315076,0.00023277005,0.0003243496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006969644,0.000012935158,0.9814184,0.000016345508,0.000019814823,0.00006890785,0.00027630042,0.00036840246,0.009834139,0.00028688152,0.00011837418,0.007509725],"study_design_scores_gemma":[0.0000015004449,0.000016343913,0.99643886,0.000002794733,0.0000056821864,0.00009322207,0.000084049585,0.0013096452,0.001629611,0.00016047196,0.00025542764,0.0000025124536],"about_ca_topic_score_codex":0.0023822475,"about_ca_topic_score_gemma":0.004048018,"teacher_disagreement_score":0.0023822475,"about_ca_system_score_codex":0.00021531802,"about_ca_system_score_gemma":0.000058392634,"threshold_uncertainty_score":0.0047367215},"labels":[],"label_agreement":null},{"id":"W2015346700","doi":"10.1088/0004-637x/791/2/87","title":"AN<i>XMM-NEWTON</i>STUDY OF THE MIXED-MORPHOLOGY SUPERNOVA REMNANT W28 (G6.4–0.1)","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Supernova remnant; Ionization; RADIUS; Astrophysics; Plasma; Ejecta; Electron temperature; Supernova; Thermal; Thermal equilibrium; Atomic physics; Thermal conduction; Ion","score_opus":0.007200733648770664,"score_gpt":0.222887371208175,"score_spread":0.21568663755940434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015346700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987531,0.00016527568,0.00026405943,0.0000132487185,0.0000015560485,0.000006015873,0.00010134753,0.000018856157,0.0006766532],"genre_scores_gemma":[0.9947588,0.00013207058,0.003234522,0.00003061938,0.000008626435,0.000009184326,0.0009098429,0.000024969228,0.0008913328],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993634,0.000004740347,0.0000032976766,0.000021707869,0.000018782923,0.000015029692],"domain_scores_gemma":[0.9997718,0.000015856232,0.00008463284,0.000035301928,0.000042617394,0.00004973453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021505007,0.00034242662,0.00022980537,0.00047595592,0.00030741026,0.00031962962,0.00043242038,0.0002613545,0.00059938873],"category_scores_gemma":[0.0002495947,0.00021423165,0.00022700136,0.00024349133,0.00020766596,0.0002777448,0.00045002354,0.00025929022,0.00045688194],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033095453,0.00014553704,0.20918916,0.0000636882,0.00013965681,0.0030842542,0.00042736143,0.0008269741,0.7768642,0.0003125352,0.0002306217,0.008385125],"study_design_scores_gemma":[0.000029022402,0.0006449985,0.9331738,0.000011059744,0.000085068095,0.006170881,0.00035738424,0.003868954,0.050096933,0.00016323909,0.0053768232,0.00002184373],"about_ca_topic_score_codex":0.0025313015,"about_ca_topic_score_gemma":0.0036121306,"teacher_disagreement_score":0.0025313015,"about_ca_system_score_codex":0.00019096515,"about_ca_system_score_gemma":0.000119900724,"threshold_uncertainty_score":0.0050331354},"labels":[],"label_agreement":null},{"id":"W2015409743","doi":"10.1086/322395","title":"The Discovery of Cepheids and a New Distance to NGC 2841 Using the<i>Hubble Space Telescope</i>","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Distance modulus; Photometry (optics); Spiral galaxy; Metallicity; Hubble sequence; Galaxy","score_opus":0.01009007762824892,"score_gpt":0.2242178215582163,"score_spread":0.21412774392996736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015409743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974679,0.0004357144,0.00037705764,0.00009024528,0.0000084685435,0.0000047546964,0.00020602321,0.000020514339,0.0013893364],"genre_scores_gemma":[0.9974033,0.00029502797,0.0009266817,0.000038866983,0.000031681648,0.000004891971,0.00070065766,0.000008369899,0.00059045653],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970347,0.000028016133,0.000017316594,0.00010991221,0.00008762573,0.00005365221],"domain_scores_gemma":[0.99892837,0.00012364914,0.00040375805,0.0001247621,0.00015168343,0.00026773603],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028897953,0.00023650353,0.00023436296,0.0007723295,0.0006899876,0.0008725434,0.0003846564,0.0003367221,0.0010836482],"category_scores_gemma":[0.0012315664,0.00020075633,0.0001539788,0.0006534941,0.00052345,0.0005186,0.00080065976,0.0004891306,0.00026322427],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018051326,0.00007677873,0.9441534,0.00006863779,0.000050300696,0.001338395,0.0013193936,0.0006128563,0.025268858,0.000833206,0.00089438516,0.02520322],"study_design_scores_gemma":[0.0000056417284,0.000040886283,0.9947918,0.0000070945034,0.000014019935,0.0008403114,0.00010806118,0.00023638007,0.0007940169,0.00014799723,0.0030061915,0.0000076061974],"about_ca_topic_score_codex":0.0062166536,"about_ca_topic_score_gemma":0.011124489,"teacher_disagreement_score":0.0062166536,"about_ca_system_score_codex":0.00065334304,"about_ca_system_score_gemma":0.0002549352,"threshold_uncertainty_score":0.01236093},"labels":[],"label_agreement":null},{"id":"W2015412178","doi":"10.1088/0004-637x/694/2/1610","title":"THE YUAN-TSEH LEE ARRAY FOR MICROWAVE BACKGROUND ANISOTROPY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Cosmic microwave background; Synchrotron radiation; Galaxy; Cosmic background radiation; Interferometry; Background radiation; Microwave; Anisotropy; Subaru Telescope","score_opus":0.0113515325282225,"score_gpt":0.23296553704631634,"score_spread":0.22161400451809385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015412178","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.077839755,0.020218244,0.41749498,0.014118552,0.004521855,0.0012462431,0.047058515,0.04366027,0.3738416],"genre_scores_gemma":[0.44290853,0.004390468,0.3914194,0.0020133008,0.0031867763,0.0017913568,0.029349308,0.0021292516,0.12281158],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99930096,0.00015379068,0.000021269443,0.00020702103,0.00018888565,0.00012801122],"domain_scores_gemma":[0.9982817,0.0001747483,0.0001510415,0.00042752767,0.00043872473,0.00052620017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019077274,0.0006725182,0.00058635167,0.0019595313,0.00092208525,0.00096345606,0.00064752845,0.0005247286,0.048154928],"category_scores_gemma":[0.0014447984,0.00037266308,0.00037782444,0.001143941,0.00030311613,0.0010081682,0.0020576203,0.0014191808,0.017235724],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009869975,0.00020539832,0.030967169,0.0002922629,0.00021453164,0.0006545898,0.0002611881,0.0011824722,0.07118298,0.029174794,0.40040788,0.46446976],"study_design_scores_gemma":[0.0005846851,0.00037022584,0.06837261,0.00010222799,0.00015656737,0.0017285954,0.00009424926,0.01685068,0.016031966,0.015073469,0.8803987,0.00023608594],"about_ca_topic_score_codex":0.001346393,"about_ca_topic_score_gemma":0.0025109989,"teacher_disagreement_score":0.048154928,"about_ca_system_score_codex":0.00038669107,"about_ca_system_score_gemma":0.00085186225,"threshold_uncertainty_score":0.16109425},"labels":[],"label_agreement":null},{"id":"W2015430322","doi":"10.1088/0004-637x/746/2/188","title":"THE GEMINI CLUSTER ASTROPHYSICS SPECTROSCOPIC SURVEY (GCLASS): THE ROLE OF ENVIRONMENT AND SELF-REGULATION IN GALAXY EVOLUTION AT<i>z</i>∼ 1","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":324,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Waterloo; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência e Tecnologia; Science and Technology Facilities Council; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Galaxy cluster; Cluster (spacecraft); Galaxy; Stellar evolution; Globular cluster; Galaxy formation and evolution; Type-cD galaxy; Brightest cluster galaxy","score_opus":0.004419328248743398,"score_gpt":0.18775711122715588,"score_spread":0.1833377829784125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015430322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96331185,0.0014862412,0.0005642298,0.0018457128,0.000028756414,0.000022228824,0.013651014,0.00013316592,0.018956877],"genre_scores_gemma":[0.9873344,0.0006481487,0.0013791411,0.00018394674,0.00006125582,0.000015146661,0.0076186866,0.000035696587,0.002723603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998479,0.000027802127,0.00000709788,0.00004457477,0.000043175503,0.000029468894],"domain_scores_gemma":[0.99896324,0.00006942101,0.00045371676,0.000101919635,0.0001353919,0.00027635464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043163315,0.000106391126,0.000116280695,0.001298337,0.0005170309,0.0009752988,0.00021853672,0.00018724386,0.0019083985],"category_scores_gemma":[0.0013025568,0.00006786784,0.00007081057,0.00265299,0.0002654676,0.0006827953,0.0011170253,0.00019995587,0.00035651933],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018100717,0.000031768734,0.932951,0.00007214732,0.0000381159,0.000045757748,0.0010425089,0.00018237987,0.0035577444,0.0028595515,0.011807895,0.047230143],"study_design_scores_gemma":[0.000002064384,0.0000049959262,0.99125755,0.0000056146823,0.000005773167,0.000013090768,0.00017251783,0.00009643506,0.0001479367,0.00021313269,0.008078603,0.0000023318053],"about_ca_topic_score_codex":0.041777957,"about_ca_topic_score_gemma":0.08363694,"teacher_disagreement_score":0.041777957,"about_ca_system_score_codex":0.0007383564,"about_ca_system_score_gemma":0.00084294507,"threshold_uncertainty_score":0.08306956},"labels":[],"label_agreement":null},{"id":"W2015440952","doi":"10.1088/0004-637x/744/2/97","title":"CONSTRAINING RADIO EMISSION FROM MAGNETARS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Luminosity; Radio telescope; Telescope; Radio astronomy; Pulse (music)","score_opus":0.025587986568463547,"score_gpt":0.29277070404194216,"score_spread":0.2671827174734786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015440952","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970337,0.000512299,0.0008492855,0.000030241688,0.000008334257,0.00000625589,0.00015555164,0.000028911445,0.0013753525],"genre_scores_gemma":[0.997957,0.0001810209,0.00097432476,0.00003576233,0.000029255356,0.0000075682096,0.00051580643,0.000009590555,0.00028972805],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998147,0.000023172179,0.000010784925,0.00005333961,0.000028987744,0.00006907742],"domain_scores_gemma":[0.9992793,0.00014989315,0.00031822693,0.000050509425,0.00007001593,0.0001320161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033125115,0.00047325328,0.00035348948,0.0014571096,0.00043845607,0.0010300085,0.00041374343,0.00040664538,0.0009278003],"category_scores_gemma":[0.0006622145,0.0002872868,0.00018726295,0.00058606506,0.00024241999,0.00028726406,0.00067743595,0.00034189704,0.00046410953],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002418511,0.00006761371,0.90536726,0.00007957548,0.00007688764,0.0007815347,0.00037059435,0.00051725406,0.07696277,0.00032107523,0.00041531606,0.014798176],"study_design_scores_gemma":[0.00001835159,0.00015521761,0.99019593,0.000013981674,0.00007845818,0.0006544304,0.0002213957,0.0008013353,0.005066721,0.00016714583,0.0026113498,0.000015670534],"about_ca_topic_score_codex":0.0012230515,"about_ca_topic_score_gemma":0.0030693014,"teacher_disagreement_score":0.0014571096,"about_ca_system_score_codex":0.00020356184,"about_ca_system_score_gemma":0.00012697109,"threshold_uncertainty_score":0.0031037927},"labels":[],"label_agreement":null},{"id":"W2015461531","doi":"10.1088/0004-637x/770/2/114","title":"STELLAR POPULATIONS IN COMPACT GALAXY GROUPS: A MULTI-WAVELENGTH STUDY OF HCGs 16, 22, AND 42, THEIR STAR CLUSTERS, AND DWARF GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Western University; Herzberg Institute of Astrophysics","funders":"","keywords":"Dwarf galaxy; Galaxy; Population; Star cluster; Globular cluster; Star formation","score_opus":0.020614377452232296,"score_gpt":0.23878688658207656,"score_spread":0.21817250912984426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015461531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995679,0.000051439747,0.000045634715,0.0000051290563,3.5553165e-7,0.0000014034313,0.00003860828,0.0000017814548,0.00028774582],"genre_scores_gemma":[0.99954504,0.000024966846,0.0001426242,0.0000043953387,0.0000023442208,0.0000017553618,0.00011686922,0.0000013971202,0.00016055578],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990356,0.000011417702,0.0000064851693,0.00002911628,0.000020287067,0.000029232633],"domain_scores_gemma":[0.99961865,0.000039893686,0.00012298577,0.00003507291,0.000037069472,0.00014633448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018387221,0.00013992637,0.00015562878,0.0016571428,0.000260778,0.00040192524,0.00012868865,0.00014995832,0.00074160093],"category_scores_gemma":[0.00038809868,0.00008153542,0.00016146818,0.00089576584,0.00024768565,0.00025233225,0.0006306779,0.00014447336,0.00019598371],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000069750226,0.000016350632,0.98993087,0.0000050752865,0.000022265402,0.00007321377,0.00046263856,0.00010006984,0.004865735,0.00009861173,0.000034407014,0.0043209605],"study_design_scores_gemma":[0.00000137336,0.000021881164,0.9989637,0.0000014352049,0.000005593146,0.00013519429,0.00030926696,0.00014063402,0.00020901256,0.000048599308,0.00016205102,0.0000012353588],"about_ca_topic_score_codex":0.0031181239,"about_ca_topic_score_gemma":0.004487249,"teacher_disagreement_score":0.0031181239,"about_ca_system_score_codex":0.00018258985,"about_ca_system_score_gemma":0.000102984704,"threshold_uncertainty_score":0.006199956},"labels":[],"label_agreement":null},{"id":"W2015494003","doi":"10.1088/0004-637x/725/1/173","title":"AN OPTICAL-INFRARED STUDY OF THE YOUNG MULTIPOLAR PLANETARY NEBULA NGC 6644","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Nebula; Astrophysics; Astronomy; Reflection nebula; Bipolar nebula; Planetary nebula; Sky; Infrared; Torus; Hubble sequence; Galaxy; Stars; Spiral galaxy","score_opus":0.008001015332627903,"score_gpt":0.22552676619524786,"score_spread":0.21752575086261997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015494003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99934036,0.0000981972,0.00006207642,0.000005598308,0.0000010020791,0.0000023843118,0.000038405287,0.0000026666942,0.0004494032],"genre_scores_gemma":[0.99850935,0.00019024477,0.0005169767,0.000016705344,0.0000050396316,0.0000031395298,0.00021108885,0.000002475412,0.00054487406],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999571,0.000003530788,0.0000022772297,0.000013241194,0.00001174588,0.000012111041],"domain_scores_gemma":[0.9998814,0.000013042818,0.00003625089,0.000010562234,0.000016735512,0.000042091808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000116800446,0.00021782129,0.00014299987,0.0008225278,0.00065728807,0.00021864424,0.00015937154,0.00020874293,0.00069249945],"category_scores_gemma":[0.00013113079,0.00020755334,0.00010975635,0.0005193499,0.00023202687,0.0003064636,0.00031447364,0.00019641998,0.00019963166],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020900795,0.00030238778,0.5467394,0.00009683716,0.00007437746,0.0029771635,0.0014651965,0.0009122095,0.42712775,0.0006289316,0.00034711894,0.019119674],"study_design_scores_gemma":[0.0000053053795,0.0001141114,0.99405104,0.0000046653695,0.000015060369,0.0013127055,0.00019079416,0.00033649607,0.002626981,0.00007902057,0.001259726,0.0000040901077],"about_ca_topic_score_codex":0.004075344,"about_ca_topic_score_gemma":0.0059591336,"teacher_disagreement_score":0.004075344,"about_ca_system_score_codex":0.00022121065,"about_ca_system_score_gemma":0.00012598037,"threshold_uncertainty_score":0.008103251},"labels":[],"label_agreement":null},{"id":"W2015545718","doi":"10.1088/0004-637x/791/1/55","title":"WATER VAPOR IN THE SPECTRUM OF THE EXTRASOLAR PLANET HD 189733b. I. THE TRANSIT","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":321,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Grism; Transit (satellite); Wide Field Camera 3; Exoplanet; Water vapor; Planet; Ultraviolet; Rayleigh scattering; Hot Jupiter","score_opus":0.007165873161110674,"score_gpt":0.19294558175384538,"score_spread":0.1857797085927347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015545718","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944465,0.00016705203,0.00034599713,0.000059255628,0.0000135971295,0.000006409612,0.0029175628,0.00015882979,0.0018847147],"genre_scores_gemma":[0.9955303,0.000060922197,0.0006172054,0.00003134475,0.000011713348,0.0000062718445,0.0034152968,0.000043358963,0.00028354579],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996793,0.0000015999887,6.660992e-7,0.000011853452,0.0000071482223,0.00001073544],"domain_scores_gemma":[0.9999474,0.0000044133167,0.00001499002,0.000006166918,0.000007983242,0.000018951909],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000041379608,0.00018750523,0.00015754199,0.00051207753,0.000347015,0.00020189406,0.00017311459,0.00020238226,0.0016891371],"category_scores_gemma":[0.00007796904,0.00008404997,0.00021981962,0.00056350994,0.00018039315,0.00017935413,0.00017451789,0.00023032307,0.00033519062],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018148874,0.0003319951,0.3853021,0.00037230158,0.0002984053,0.0022252533,0.0012777173,0.0032053234,0.539938,0.0019893728,0.016990533,0.04625417],"study_design_scores_gemma":[0.000025079504,0.00007011881,0.9824327,0.00000876208,0.000036076795,0.00030898387,0.00010514201,0.0022115223,0.010132748,0.00016696335,0.004487777,0.0000141062],"about_ca_topic_score_codex":0.01218614,"about_ca_topic_score_gemma":0.019465415,"teacher_disagreement_score":0.01218614,"about_ca_system_score_codex":0.00040597396,"about_ca_system_score_gemma":0.00009253498,"threshold_uncertainty_score":0.02423042},"labels":[],"label_agreement":null},{"id":"W2015568734","doi":"10.1086/381242","title":"Theoretical Examination of the Lithium Depletion Boundary","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Pleiades; Open cluster; Cluster (spacecraft); Magnitude (astronomy); Star cluster; Rotation (mathematics); Stellar rotation; Ionization","score_opus":0.006660143209672923,"score_gpt":0.21125195040083405,"score_spread":0.20459180719116113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015568734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.48673612,0.0016690689,0.1939312,0.0046473127,0.00017397827,0.00008931569,0.0006461335,0.00089545245,0.31121138],"genre_scores_gemma":[0.9881566,0.0003067787,0.007104407,0.00022499077,0.000052741692,0.00006652897,0.00014856397,0.00008028508,0.0038589393],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997285,0.000052983683,0.0000075696366,0.000067928995,0.000071250106,0.00007170504],"domain_scores_gemma":[0.99898785,0.0004902926,0.00014518062,0.0001162909,0.00014361023,0.000116787465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010845677,0.00039742104,0.00051811454,0.001157343,0.0009998584,0.001553571,0.0023495147,0.0011597809,0.0071387086],"category_scores_gemma":[0.005552181,0.00037394173,0.00053112174,0.0004380009,0.0018126976,0.0030127643,0.0024577114,0.00096611393,0.00090614124],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000680134,0.000033259592,0.005023857,0.00008643418,0.000013051489,0.00030919563,0.00041855656,0.08449735,0.0016925969,0.8979193,0.0013438129,0.008594524],"study_design_scores_gemma":[0.000036567784,0.000050747123,0.0019886624,0.00006750952,0.000012233882,0.00018864933,0.00015614409,0.5409696,0.0016242309,0.44919673,0.005667928,0.00004104798],"about_ca_topic_score_codex":0.0029513766,"about_ca_topic_score_gemma":0.0011101173,"teacher_disagreement_score":0.0071387086,"about_ca_system_score_codex":0.0018104935,"about_ca_system_score_gemma":0.00068161695,"threshold_uncertainty_score":0.023881316},"labels":[],"label_agreement":null},{"id":"W2015645360","doi":"10.1088/0004-637x/796/2/90","title":"THE CARINA PROJECT. VII. TOWARD THE BREAKING OF THE AGE-METALLICITY DEGENERACY OF RED GIANT BRANCH STARS USING THE<i>C</i><sub>U, B, I</sub>INDEX","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Red-giant branch; Stars; Globular cluster; Degeneracy (biology); Horizontal branch; RGB color model; Asymptotic giant branch; Population; Star count","score_opus":0.017114626700949497,"score_gpt":0.2366763943626425,"score_spread":0.21956176766169302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015645360","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.35782978,0.057029184,0.065381534,0.012513825,0.0017065818,0.0009522385,0.24170598,0.03288259,0.22999822],"genre_scores_gemma":[0.5300014,0.0068054,0.13452761,0.002641177,0.00072121364,0.0011295297,0.2384904,0.006605173,0.07907806],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99914384,0.00018300531,0.000030055344,0.00028677084,0.0002190456,0.00013726413],"domain_scores_gemma":[0.998384,0.0001802176,0.0002492369,0.00033440377,0.00055476,0.00029744726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021387476,0.0011932139,0.00058510894,0.0022987025,0.0005905894,0.0027789078,0.0012243737,0.0008920731,0.0060980273],"category_scores_gemma":[0.002635805,0.00034332523,0.0004043724,0.001323306,0.00046359195,0.0011698366,0.0023649007,0.0005792955,0.0060697934],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0034339398,0.00024013205,0.15564254,0.0014537345,0.00048457723,0.00053145585,0.0014042329,0.0035340914,0.009277914,0.026614573,0.20555952,0.59182334],"study_design_scores_gemma":[0.00032762738,0.00020991219,0.15447052,0.0005771509,0.0002445823,0.00061923516,0.0006358925,0.0084959855,0.007993752,0.013055691,0.813283,0.000086548906],"about_ca_topic_score_codex":0.030584374,"about_ca_topic_score_gemma":0.025527727,"teacher_disagreement_score":0.030584374,"about_ca_system_score_codex":0.0013324649,"about_ca_system_score_gemma":0.0013083646,"threshold_uncertainty_score":0.06081271},"labels":[],"label_agreement":null},{"id":"W2015698171","doi":"10.1086/503869","title":"The Extended H <scp>i</scp> Rotation Curve and Mass Distribution of M31","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Galaxy rotation curve; Mass distribution; Physics; Galaxy; Astrophysics; Mass ratio; Rotation (mathematics); Light curve; Astronomy; Geometry; Galaxy formation and evolution; Mathematics","score_opus":0.004525893962053537,"score_gpt":0.2004832816578449,"score_spread":0.19595738769579135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015698171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929438,0.00010589161,0.00021451367,0.00013054785,0.0000051355655,0.000005505135,0.0012404779,0.000026111762,0.0053280136],"genre_scores_gemma":[0.99752337,0.000036684647,0.000079011785,0.000024037785,0.000014614971,0.0000029219073,0.0012557275,0.000009787832,0.0010538702],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995065,0.0000049128257,0.0000017019448,0.000015838346,0.0000067230208,0.000020248513],"domain_scores_gemma":[0.9995474,0.00006979974,0.000097409364,0.000038672788,0.000083783576,0.00016292352],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019082117,0.00014791121,0.00013359926,0.0008988831,0.00033838177,0.00036392699,0.00016541948,0.0002916727,0.008732624],"category_scores_gemma":[0.00053368014,0.00009742874,0.00012225524,0.00066737743,0.0001827919,0.0003844194,0.00036735923,0.00022232327,0.0020578885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063141284,0.00006697625,0.92115474,0.000036453865,0.000031555686,0.00041419396,0.00066836807,0.001365769,0.03465625,0.0015972393,0.0054229847,0.03395396],"study_design_scores_gemma":[0.0000036887752,0.000021159685,0.9983589,0.0000019791344,0.0000023346429,0.00007275901,0.000060488874,0.0003265722,0.00021576048,0.00014408964,0.00078956905,0.000002631953],"about_ca_topic_score_codex":0.0039753024,"about_ca_topic_score_gemma":0.004558671,"teacher_disagreement_score":0.008732624,"about_ca_system_score_codex":0.0002348056,"about_ca_system_score_gemma":0.00014581723,"threshold_uncertainty_score":0.029213488},"labels":[],"label_agreement":null},{"id":"W2015737155","doi":"10.1086/340561","title":"Nobeyama Millimeter Array CO (<i>J</i> = 1–0) Observations of the Hα/Radio Lobe Galaxy NGC 3079: Gas Dynamics in a Weak Bar Potential and Central Massive Core","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; RADIUS; Spiral galaxy; Millimeter; Galaxy; Bar (unit); Spiral (railway); Submillimeter Array; Core (optical fiber); Astronomy; Star formation; Optics","score_opus":0.010385331657658661,"score_gpt":0.19429273350836954,"score_spread":0.18390740185071086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015737155","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99728477,0.000052712974,0.00017162749,0.00002628323,0.0000038566536,0.0000040179143,0.0003512382,0.000028563745,0.002076969],"genre_scores_gemma":[0.9986249,0.000033253873,0.0004097912,0.000016358556,0.0000069928487,0.0000055072423,0.0005039398,0.000004909336,0.00039434445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993885,0.000004603443,0.0000025134163,0.000018221648,0.000016402668,0.000019319858],"domain_scores_gemma":[0.9997962,0.0000136087765,0.000056747056,0.00002237285,0.000018367882,0.00009272457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000079158424,0.00013487876,0.00018378353,0.00042392436,0.0002787428,0.0002346684,0.00024054422,0.00023655563,0.0017799514],"category_scores_gemma":[0.00013600689,0.00012214301,0.000104016755,0.0003347496,0.00015066766,0.00015281847,0.0003670095,0.0002051786,0.0006236141],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032403972,0.00009255129,0.8599886,0.00005531689,0.000051665458,0.0013651199,0.00031619033,0.0005800409,0.12127506,0.0003340873,0.002442583,0.013174773],"study_design_scores_gemma":[0.000008403733,0.000035692487,0.99594927,0.0000060303378,0.000013096441,0.00036924047,0.00009089008,0.0005892146,0.0018402546,0.00005350903,0.0010398814,0.0000044578205],"about_ca_topic_score_codex":0.0053923954,"about_ca_topic_score_gemma":0.01723688,"teacher_disagreement_score":0.0053923954,"about_ca_system_score_codex":0.00018086955,"about_ca_system_score_gemma":0.00011808303,"threshold_uncertainty_score":0.010722041},"labels":[],"label_agreement":null},{"id":"W2015836516","doi":"10.1086/308267","title":"An Observational Test of Dark Matter as Cold Fractal Clouds","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Scientific Research and Discoveries","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Dark matter; Galaxy; Galaxy rotation curve; Quasar; Halo; RADIUS; Astronomy; Dark matter halo; Dark galaxy","score_opus":0.02205724330961592,"score_gpt":0.2925173774410051,"score_spread":0.27046013413138914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015836516","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931988,0.00013627495,0.0025556453,0.00032526185,0.000008694369,0.0000070406936,0.00015835512,0.00003406965,0.0035758766],"genre_scores_gemma":[0.9992924,0.000017385675,0.00049728603,0.000043097596,0.000007029447,0.0000024113863,0.0000577147,0.0000018405035,0.000080833976],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995616,0.00011690225,0.000020753081,0.00007931811,0.000110962166,0.00011044001],"domain_scores_gemma":[0.9915937,0.0037940156,0.0017663778,0.0013090278,0.0005123831,0.0010245043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011893333,0.00010684996,0.00023184132,0.00064878457,0.0004139926,0.0005586359,0.00039767855,0.00038172505,0.0012531637],"category_scores_gemma":[0.0058003594,0.00011519188,0.00015958856,0.00044037678,0.0016836205,0.0010241595,0.001109981,0.0005151277,0.000090494665],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000610915,0.00010968019,0.89845353,0.000088092784,0.000114000526,0.0005318555,0.0012857463,0.0022204362,0.030628392,0.045392986,0.0011006575,0.019463632],"study_design_scores_gemma":[0.00010423326,0.00034781103,0.9039757,0.00007807574,0.00003989735,0.0011082772,0.0014123016,0.01660691,0.009266514,0.060751967,0.006233486,0.00007470401],"about_ca_topic_score_codex":0.0017657427,"about_ca_topic_score_gemma":0.0013909255,"teacher_disagreement_score":0.0017657427,"about_ca_system_score_codex":0.00041542447,"about_ca_system_score_gemma":0.00022278205,"threshold_uncertainty_score":0.0062898993},"labels":[],"label_agreement":null},{"id":"W2015955391","doi":"10.1086/422676","title":"Extended Molecular Gas in the Nearby Starburst Galaxy Maffei 2","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Dwarf galaxy; Spiral galaxy; Galaxy rotation curve; Bar (unit); Star formation; Molecular cloud; Stars","score_opus":0.005717039865570423,"score_gpt":0.21131129266715645,"score_spread":0.20559425280158602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2015955391","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983096,0.00020079222,0.00017610482,0.000027305798,0.0000025020447,0.0000036525832,0.00024093456,0.000018461391,0.0010207354],"genre_scores_gemma":[0.99858785,0.000102039936,0.0004989302,0.000012559704,0.000009647307,0.0000060973284,0.00053803355,0.0000035963435,0.00024128113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999479,0.000004816444,0.0000023014297,0.000020675508,0.00000905352,0.00001533357],"domain_scores_gemma":[0.99979144,0.000032449247,0.00006379519,0.000023440532,0.000018848525,0.00007005235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009562058,0.00016651269,0.00017639427,0.0011458107,0.000316707,0.00043333377,0.00028973265,0.00023950067,0.0010609173],"category_scores_gemma":[0.00036684112,0.00013785271,0.00015332595,0.00049665786,0.00018720816,0.00025504243,0.0005815806,0.00016644347,0.00014788979],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031445018,0.000102576254,0.8949729,0.00006558059,0.00009667702,0.0009890525,0.0016231315,0.002108131,0.07384469,0.0008577178,0.00089245324,0.024132553],"study_design_scores_gemma":[0.00000718344,0.000040625535,0.9959996,0.000009337361,0.000011966276,0.00031076383,0.00011748787,0.0009151837,0.00079387095,0.00013797863,0.0016503095,0.0000056956446],"about_ca_topic_score_codex":0.005413651,"about_ca_topic_score_gemma":0.0097802365,"teacher_disagreement_score":0.005413651,"about_ca_system_score_codex":0.00029076397,"about_ca_system_score_gemma":0.000092356204,"threshold_uncertainty_score":0.010764301},"labels":[],"label_agreement":null},{"id":"W2016005396","doi":"10.1086/422137","title":"The Gas‐Phase Formation of Methyl Formate in Hot Molecular Cores","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":157,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Wilfrid Laurier University","funders":"","keywords":"Methyl formate; Formate; Molecule; Methanol; Formaldehyde; Protonation; Ion; Chemical reaction; Photochemistry; Mass spectrum; Physics; Chemistry; Chemical physics; Organic chemistry; Catalysis","score_opus":0.004978729655328644,"score_gpt":0.255225405706951,"score_spread":0.2502466760516224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016005396","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948043,0.00044608567,0.002234498,0.0000398123,0.00000862772,0.000015751664,0.00010560247,0.000029678311,0.002315538],"genre_scores_gemma":[0.999067,0.000116565054,0.00039187557,0.00000877925,0.0000029426944,0.000004107878,0.00007244843,0.0000034118439,0.0003327242],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999933,0.0000072724424,0.0000015628018,0.000015626743,0.000018513769,0.000024017183],"domain_scores_gemma":[0.9998752,0.00004258966,0.000033231492,0.00001819231,0.000014449073,0.000016381786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018030543,0.00024284727,0.00016927657,0.0002504051,0.0003373263,0.00031414191,0.00042468111,0.00043606412,0.0014640292],"category_scores_gemma":[0.00034786426,0.00020273087,0.00016950787,0.00014309071,0.00050069916,0.0005599521,0.00025656575,0.00025424073,0.00019513065],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059485406,0.00010022389,0.01213633,0.00025014608,0.00004050539,0.00058528635,0.00022773758,0.0049009565,0.9666995,0.008595383,0.00021043612,0.0056586987],"study_design_scores_gemma":[0.000112988564,0.00050745165,0.02751145,0.000016197211,0.00002572481,0.0003207912,0.00018913219,0.020623775,0.9451054,0.0036571675,0.0019075206,0.000022408174],"about_ca_topic_score_codex":0.0010667848,"about_ca_topic_score_gemma":0.0006638732,"teacher_disagreement_score":0.0014640292,"about_ca_system_score_codex":0.0004064301,"about_ca_system_score_gemma":0.00013424184,"threshold_uncertainty_score":0.0048977137},"labels":[],"label_agreement":null},{"id":"W2016072621","doi":"10.1088/0004-637x/760/1/75","title":"THE PAL 5 STAR STREAM GAPS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Halo; Globular cluster; Sky; Astrophysics; Population; Cluster (spacecraft); Stars; Galaxy","score_opus":0.007240039966614402,"score_gpt":0.21268690582172492,"score_spread":0.20544686585511052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016072621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97159404,0.000091397524,0.0069992095,0.00011287046,0.00004073902,0.000041683885,0.005538209,0.0011250781,0.014456757],"genre_scores_gemma":[0.9878088,0.000021625709,0.005417881,0.00005293251,0.000007565082,0.000024820756,0.005395917,0.000095946256,0.0011744661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995957,0.000052651372,0.000018351173,0.00011630308,0.00013989377,0.00007709829],"domain_scores_gemma":[0.9989786,0.00023853229,0.00020965333,0.00022637387,0.00018745195,0.00015948185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046276322,0.00022454628,0.0002509675,0.00048551158,0.0005220417,0.00079269474,0.00050834136,0.00031789983,0.0049208803],"category_scores_gemma":[0.0027509546,0.00016890671,0.00031769258,0.00057022576,0.00029734324,0.0005558006,0.0008748481,0.00039226757,0.0011188249],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010721335,0.0003122116,0.82342803,0.00020726299,0.00011381069,0.0009469922,0.0010664728,0.029793566,0.01423706,0.01669149,0.032675065,0.0794558],"study_design_scores_gemma":[0.00013216549,0.0005666994,0.69054663,0.00013368503,0.000087628556,0.0015489148,0.0008206878,0.19761679,0.026426168,0.0122390855,0.0698112,0.00007031181],"about_ca_topic_score_codex":0.003693439,"about_ca_topic_score_gemma":0.004233571,"teacher_disagreement_score":0.0049208803,"about_ca_system_score_codex":0.00044238483,"about_ca_system_score_gemma":0.00042348288,"threshold_uncertainty_score":0.016461968},"labels":[],"label_agreement":null},{"id":"W2016096905","doi":"10.1088/0004-637x/794/2/159","title":"A STATISTICAL ANALYSIS OF SEEDS AND OTHER HIGH-CONTRAST EXOPLANET SURVEYS: MASSIVE PLANETS OR LOW-MASS BROWN DWARFS?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Physics; Exoplanet; Planet; Stars; Astrophysics; Pleiades; Sky; Astronomy","score_opus":0.009642403679176232,"score_gpt":0.22517083051725656,"score_spread":0.21552842683808032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016096905","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9873324,0.00014705792,0.009675294,0.0001198264,0.000029693812,0.00007792243,0.0016855324,0.00011007944,0.0008222039],"genre_scores_gemma":[0.99393624,0.000030239938,0.0029241224,0.000040963747,0.00003943595,0.00006600463,0.002430333,0.000061905055,0.0004708783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.98995656,0.003951754,0.00092617114,0.002295574,0.0020607496,0.000809186],"domain_scores_gemma":[0.94673747,0.037280988,0.005747632,0.0061047953,0.00207144,0.002057696],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010464908,0.000602444,0.0009988096,0.0035744724,0.0007732773,0.0013551951,0.001209137,0.00074711785,0.0028484494],"category_scores_gemma":[0.03441699,0.00027299087,0.0016127158,0.0028663203,0.0016214927,0.0014596302,0.001165787,0.0009285587,0.0006312955],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010688076,0.00015953893,0.97192377,0.00006930462,0.0014075054,0.000470022,0.00023842977,0.0012239189,0.004562075,0.0010818926,0.0017575722,0.016037207],"study_design_scores_gemma":[0.00009652913,0.0015735197,0.9598443,0.000022553068,0.00079051853,0.00133552,0.00094498106,0.027425412,0.0029651728,0.0012182688,0.0037358853,0.000047237318],"about_ca_topic_score_codex":0.0024279554,"about_ca_topic_score_gemma":0.0022904247,"teacher_disagreement_score":0.010464908,"about_ca_system_score_codex":0.0003958204,"about_ca_system_score_gemma":0.0007549842,"threshold_uncertainty_score":0.055344403},"labels":[],"label_agreement":null},{"id":"W2016258946","doi":"10.1086/519445","title":"Star Formation at Very Low Metallicity. I. Chemistry and Cooling at Low Densities","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":184,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Metallicity; Thermal; Hydrogen; Ultraviolet; Chemistry; Hydrogen molecule; Physics; Physical chemistry; Astrophysics; Thermodynamics; Quantum mechanics; Stars; Organic chemistry","score_opus":0.007346475450659895,"score_gpt":0.21668061355200402,"score_spread":0.20933413810134413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016258946","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8559541,0.0038019929,0.091196835,0.002695378,0.00018721838,0.00017633825,0.0014844646,0.00069907546,0.043804504],"genre_scores_gemma":[0.986785,0.0011492391,0.004583065,0.00024679917,0.00009175154,0.00008123699,0.00033769285,0.000077595876,0.0066475947],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986386,0.000030498655,0.0000054244783,0.000031883344,0.000026035634,0.000042265],"domain_scores_gemma":[0.99972683,0.00005164441,0.000075825315,0.000052395993,0.00003414135,0.00005925721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022779121,0.0007711183,0.0009664798,0.00038022964,0.00082735985,0.0011884855,0.0014682317,0.0016606704,0.0026114613],"category_scores_gemma":[0.0011735389,0.0004995372,0.000853732,0.00034266515,0.0016041495,0.00201741,0.0010788311,0.0006586318,0.00083352375],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013351825,0.00010989124,0.020574817,0.00032778914,0.00006716152,0.0007054492,0.00038391436,0.77972823,0.020694563,0.16698463,0.002353833,0.007936159],"study_design_scores_gemma":[0.00012645437,0.00012254952,0.010944407,0.000035517925,0.0000318823,0.00043285458,0.00008512753,0.8571033,0.002437359,0.12330529,0.0053368425,0.000038324564],"about_ca_topic_score_codex":0.007298137,"about_ca_topic_score_gemma":0.002748363,"teacher_disagreement_score":0.007298137,"about_ca_system_score_codex":0.0015786791,"about_ca_system_score_gemma":0.000551185,"threshold_uncertainty_score":0.014511347},"labels":[],"label_agreement":null},{"id":"W2016277399","doi":"10.1088/0004-637x/750/1/37","title":"COSMOS: STOCHASTIC BIAS FROM MEASUREMENTS OF WEAK LENSING AND GALAXY CLUSTERING","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Galaxy; Halo; Weak gravitational lensing; Satellite galaxy; Redshift; Dark matter; Galaxy rotation curve; Correlation function (quantum field theory); Galaxy formation and evolution","score_opus":0.03440336931571534,"score_gpt":0.2351779442444195,"score_spread":0.20077457492870418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016277399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90631783,0.0011367309,0.068123855,0.0003718504,0.000069563845,0.00007643687,0.015583012,0.0022503946,0.006070297],"genre_scores_gemma":[0.965721,0.0002461902,0.020400923,0.00010493943,0.00006894025,0.000070931324,0.012220815,0.00040882282,0.00075754046],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99883705,0.0004947962,0.00006827761,0.00020939963,0.00030643793,0.0000840183],"domain_scores_gemma":[0.995237,0.0016851465,0.0013405491,0.00110415,0.00038002117,0.00025315108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0037419687,0.00043769542,0.00039174367,0.0014873353,0.0003075105,0.00081544794,0.00047609,0.00034036915,0.0019269054],"category_scores_gemma":[0.009256007,0.00020645418,0.0003498079,0.0022831114,0.0005516599,0.00091499544,0.0010662108,0.00039074,0.000539347],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036800848,0.0000362107,0.9311584,0.000120304365,0.00034640435,0.000111676985,0.00019981654,0.012733908,0.0037200875,0.010301362,0.006134364,0.0347695],"study_design_scores_gemma":[0.00008578556,0.000106890024,0.8848913,0.000041824416,0.00012629724,0.00062485633,0.00014874413,0.067184925,0.0077909897,0.019427994,0.019486282,0.00008421109],"about_ca_topic_score_codex":0.0075149257,"about_ca_topic_score_gemma":0.0058960975,"teacher_disagreement_score":0.0075149257,"about_ca_system_score_codex":0.00042891825,"about_ca_system_score_gemma":0.0005051189,"threshold_uncertainty_score":0.019789636},"labels":[],"label_agreement":null},{"id":"W2016290928","doi":"10.1086/341190","title":"Normal Modes of Rotating Magnetic Stars","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Magnetic field; Magnetohydrodynamic drive; Magnetohydrodynamics; Magnetic dipole; Dipole; Perturbation (astronomy); Oscillation (cell signaling); Normal mode","score_opus":0.008116411120030843,"score_gpt":0.20271579704981366,"score_spread":0.19459938592978282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016290928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9544888,0.0003618007,0.036302075,0.00016204316,0.00007466048,0.000021928608,0.000026965346,0.00011739974,0.008444401],"genre_scores_gemma":[0.99325246,0.00025894665,0.0039918893,0.000022728105,0.00006019785,0.000010037855,0.000028934523,0.00003867704,0.0023361952],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999182,0.000025380401,0.000003181071,0.000013168409,0.000022338205,0.000017704457],"domain_scores_gemma":[0.9996289,0.000072441355,0.00010717212,0.0000304687,0.00007521826,0.0000858995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002863849,0.0005156496,0.00033035927,0.00040772738,0.00036192287,0.0004943129,0.0003583999,0.00031139952,0.0013634474],"category_scores_gemma":[0.001430692,0.00016037507,0.00026041502,0.00016629182,0.00060966687,0.0006428776,0.00069901865,0.0003639169,0.00027383913],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086487323,0.0001629281,0.026131896,0.00035071053,0.00009736711,0.0014073781,0.0026853173,0.3403518,0.21510912,0.35146126,0.0027970748,0.058580294],"study_design_scores_gemma":[0.000095657175,0.00034789136,0.010910691,0.000022410213,0.000025561068,0.00044168407,0.0003220161,0.90073884,0.010664893,0.07291664,0.0034629307,0.00005081719],"about_ca_topic_score_codex":0.0013461213,"about_ca_topic_score_gemma":0.0006504042,"teacher_disagreement_score":0.0013634474,"about_ca_system_score_codex":0.00026179192,"about_ca_system_score_gemma":0.00018287296,"threshold_uncertainty_score":0.004561186},"labels":[],"label_agreement":null},{"id":"W2016390626","doi":"10.1088/0004-637x/756/1/78","title":"A POPULATION OF NON-RECYCLED PULSARS ORIGINATING IN GLOBULAR CLUSTERS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Globular cluster; Pulsar; Millisecond pulsar; Galaxy; Supernova; Population","score_opus":0.010553840985308942,"score_gpt":0.3285213537005661,"score_spread":0.3179675127152572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016390626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976609,0.00006884334,0.001354824,0.00006816678,0.000002788134,0.000010960916,0.00007801225,0.000012573825,0.00074296055],"genre_scores_gemma":[0.9981779,0.000099256,0.0008685764,0.000028842254,0.0000042610623,0.000010427679,0.00014824403,0.000005637663,0.00065677986],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998708,0.000021750044,0.000004106214,0.00005386084,0.000015900672,0.0000336633],"domain_scores_gemma":[0.99955374,0.0001330487,0.00010661248,0.000063300344,0.00004464226,0.00009854224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039134556,0.00028802973,0.0002850917,0.00048143812,0.000778155,0.0009535745,0.001184536,0.0007293427,0.0018269749],"category_scores_gemma":[0.0012092026,0.00016575659,0.0004713772,0.00056178035,0.0010884274,0.0010195174,0.000944682,0.00038534586,0.00020701713],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031421141,0.0002795834,0.49933076,0.000115115196,0.00016390481,0.0013241159,0.0017734534,0.4479226,0.0072669336,0.023366617,0.0014490065,0.016693683],"study_design_scores_gemma":[0.00021904153,0.00080766017,0.29727417,0.000076281445,0.00020202655,0.0010046782,0.0024742454,0.6685884,0.0018315039,0.023521833,0.0038837185,0.00011653394],"about_ca_topic_score_codex":0.010539265,"about_ca_topic_score_gemma":0.008070911,"teacher_disagreement_score":0.010539265,"about_ca_system_score_codex":0.00063631916,"about_ca_system_score_gemma":0.0004992611,"threshold_uncertainty_score":0.02095586},"labels":[],"label_agreement":null},{"id":"W2016474295","doi":"10.1088/0004-637x/789/1/24","title":"COMPARING M31 AND MILKY WAY SATELLITES: THE EXTENDED STAR FORMATION HISTORIES OF ANDROMEDA II AND ANDROMEDA XVI","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Andromeda; Physics; Astrophysics; Milky Way; Galaxy; Star formation; Local Group; Andromeda Galaxy; Reionization; Astronomy; Stellar mass; Satellite galaxy; Context (archaeology); Paleontology; Geology; Redshift","score_opus":0.009654867954170511,"score_gpt":0.20073309197129224,"score_spread":0.19107822401712174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016474295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985423,0.00018932887,0.00004592586,0.000008617856,9.2185934e-7,0.0000028481238,0.00016133113,0.0000034433951,0.0010452821],"genre_scores_gemma":[0.9988306,0.00011354947,0.00013431454,0.0000084394505,0.0000031485467,0.000002879314,0.0006065179,0.0000032150738,0.00029729327],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990964,0.0000105608815,0.000004563036,0.000032356013,0.000017165412,0.000025796488],"domain_scores_gemma":[0.9996182,0.000047258975,0.0001399782,0.000039245104,0.00004293706,0.000112326525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016205879,0.00017625003,0.00015022968,0.0009355115,0.00034030573,0.0004567134,0.00017205712,0.00020146946,0.0011536601],"category_scores_gemma":[0.00057447073,0.00009896268,0.00016596407,0.0006222771,0.00020740338,0.00035258598,0.0006892997,0.00017189299,0.00031315244],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020215721,0.000019282077,0.97085327,0.000040894112,0.0000775008,0.0002303039,0.0016276531,0.0004637577,0.015140242,0.00038678554,0.00016874043,0.010789386],"study_design_scores_gemma":[0.0000022076906,0.000039895313,0.99781644,0.00000416234,0.000006939149,0.00020494235,0.00024862387,0.00012881756,0.0004453839,0.000047176538,0.0010521587,0.0000033360861],"about_ca_topic_score_codex":0.0065902714,"about_ca_topic_score_gemma":0.009547231,"teacher_disagreement_score":0.0065902714,"about_ca_system_score_codex":0.00032829182,"about_ca_system_score_gemma":0.00017433577,"threshold_uncertainty_score":0.013103843},"labels":[],"label_agreement":null},{"id":"W2016537330","doi":"10.1088/0004-637x/745/2/183","title":"CARMA SURVEY TOWARD INFRARED-BRIGHT NEARBY GALAXIES (STING). II. MOLECULAR GAS STAR FORMATION LAW AND DEPLETION TIME ACROSS THE BLUE SEQUENCE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia","funders":"","keywords":"Astrophysics; Physics; Star formation; Galaxy; Surface brightness; Power law; Infrared; Astronomy","score_opus":0.017849075465619247,"score_gpt":0.25730259093114,"score_spread":0.23945351546552074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016537330","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99282736,0.00029133234,0.0002411267,0.000045828445,0.0000052830906,0.00002159469,0.0040695337,0.0000564458,0.0024413825],"genre_scores_gemma":[0.9900366,0.0001929189,0.0010719204,0.000045275585,0.000014280996,0.000031435506,0.0062872777,0.000010880398,0.0023093522],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987686,0.000012973635,0.000005600063,0.000038703984,0.00002869392,0.000037146216],"domain_scores_gemma":[0.99929464,0.00004626994,0.00026497926,0.00007642415,0.00013937325,0.00017838557],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026058118,0.0001785399,0.00015800248,0.0018368808,0.0003134918,0.0002627376,0.00033217174,0.0001872103,0.0023750146],"category_scores_gemma":[0.0006943756,0.00012193414,0.00016325506,0.0009894143,0.00014077056,0.000276425,0.00031685774,0.0002169938,0.00080920284],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010702576,0.000040097246,0.98365915,0.000031938507,0.000029108976,0.00007296963,0.00028172747,0.000102120204,0.0034374744,0.00014104677,0.0012543638,0.010842861],"study_design_scores_gemma":[0.000002440365,0.000025388335,0.9982981,0.00000300676,0.00000797024,0.00007468325,0.000051800893,0.00015484296,0.00017356132,0.000012537729,0.0011945213,0.0000012909217],"about_ca_topic_score_codex":0.03270141,"about_ca_topic_score_gemma":0.08763387,"teacher_disagreement_score":0.03270141,"about_ca_system_score_codex":0.0004779379,"about_ca_system_score_gemma":0.00028142487,"threshold_uncertainty_score":0.06502211},"labels":[],"label_agreement":null},{"id":"W2016652538","doi":"10.1086/375482","title":"Large Mixing Angle Oscillations as a Probe of the Deep Solar Interior","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Helioseismology; Neutrino oscillation; Solar neutrino; Neutrino; Oscillation (cell signaling); Solar neutrino problem; Radiative transfer; Standard solar model","score_opus":0.013181254603241583,"score_gpt":0.27607393967748817,"score_spread":0.26289268507424657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016652538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9861426,0.00061205256,0.009800768,0.00014989484,0.00002168363,0.0000032076582,0.00010905508,0.00008205676,0.0030787017],"genre_scores_gemma":[0.99759704,0.00014110266,0.001897178,0.000032745003,0.0000135296195,0.000002094063,0.000087384244,0.000017621733,0.00021121843],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99990284,0.000024588691,0.000004001949,0.000033670127,0.000021350254,0.000013524985],"domain_scores_gemma":[0.9994467,0.00019692557,0.0001458529,0.00012672828,0.0000343565,0.0000495216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004341425,0.00023957352,0.00020922715,0.00050365855,0.00018132695,0.0004919309,0.00019096205,0.0003198235,0.00066562777],"category_scores_gemma":[0.001392154,0.00015035635,0.00016738902,0.00042446356,0.00031208605,0.0006331297,0.0006101694,0.00073167,0.000137357],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073709857,0.00012980298,0.36696497,0.00011501882,0.00029330608,0.0003491182,0.00072943023,0.0115278065,0.54476845,0.016019328,0.0005695221,0.057796158],"study_design_scores_gemma":[0.000071870505,0.0004474612,0.7734546,0.00003550445,0.00018699837,0.00084150676,0.0003545588,0.06692245,0.10708608,0.043128923,0.007390045,0.00008004586],"about_ca_topic_score_codex":0.00025814865,"about_ca_topic_score_gemma":0.0005687629,"teacher_disagreement_score":0.00066562777,"about_ca_system_score_codex":0.000104688326,"about_ca_system_score_gemma":0.000047913152,"threshold_uncertainty_score":0.0022960305},"labels":[],"label_agreement":null},{"id":"W2016698275","doi":"10.1088/0004-637x/741/2/112","title":"MULTI-SCALE ANALYSIS OF MAGNETIC FIELDS IN FILAMENTARY MOLECULAR CLOUDS IN ORION A","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université du Québec à Montréal","funders":"","keywords":"Magnetic field; Polarization (electrochemistry); Molecular cloud; Stars; Position angle; Linear polarization; Line-of-sight; Offset (computer science)","score_opus":0.013122333882928808,"score_gpt":0.23721546462455856,"score_spread":0.22409313074162976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016698275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99947816,0.000042052412,0.00015182773,0.000009148763,0.0000019010962,0.0000018600368,0.00007632419,0.0000092702185,0.00022948992],"genre_scores_gemma":[0.9995123,0.000019779103,0.00025901696,0.0000036660872,0.000004882253,0.0000026089563,0.00014132854,0.0000028693212,0.00005349003],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999205,0.0000088772,0.0000045486086,0.000029609952,0.000014881437,0.000021534057],"domain_scores_gemma":[0.9995952,0.000049724043,0.00015929913,0.00003231171,0.00005483506,0.00010866159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012635416,0.0001581508,0.00016361596,0.0014069336,0.00034795632,0.00028171722,0.00023454583,0.00017278561,0.00060853135],"category_scores_gemma":[0.00038248015,0.0001083309,0.0001546834,0.00069817685,0.00018164104,0.00021878,0.000411429,0.0001859495,0.00009338678],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000498513,0.00011885228,0.78023785,0.0000611861,0.0001567582,0.00093089516,0.0005709356,0.0022065116,0.19478808,0.00022496242,0.00023610152,0.019969333],"study_design_scores_gemma":[0.0000035367186,0.000023658884,0.9967597,0.0000026399548,0.000015612548,0.00008499498,0.00008830303,0.0015110564,0.0013022133,0.00003011861,0.00017440187,0.0000038444027],"about_ca_topic_score_codex":0.0029470497,"about_ca_topic_score_gemma":0.003570397,"teacher_disagreement_score":0.0029470497,"about_ca_system_score_codex":0.00023025279,"about_ca_system_score_gemma":0.000095335876,"threshold_uncertainty_score":0.005859792},"labels":[],"label_agreement":null},{"id":"W2016725966","doi":"10.1086/590339","title":"IRAS 04325+2402C: A Very Low Mass Object with an Edge-On Disk","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Protostar; Photometry (optics); Spectral energy distribution; Low Mass; Young stellar object; Photosphere; Radiative transfer; Astronomy; Millimeter; Infrared; Brown dwarf; Star formation; Stars; Spectral line; Optics; Galaxy","score_opus":0.01039938414945775,"score_gpt":0.22256023259660562,"score_spread":0.2121608484471479,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016725966","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921095,0.00025525477,0.00058203994,0.00010176085,0.00001953989,0.000020818617,0.00052129803,0.00015320991,0.0062366105],"genre_scores_gemma":[0.9961712,0.000032608703,0.000985539,0.00008628371,0.000030779258,0.000009515537,0.001267708,0.000016837868,0.0013996289],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981576,0.000009811428,0.000009877127,0.000047297894,0.00005279975,0.00006444155],"domain_scores_gemma":[0.9996855,0.000016477867,0.000087808025,0.000035413253,0.00003209136,0.0001426731],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020403284,0.00052016514,0.0003122688,0.0014220705,0.0010730221,0.0006613872,0.00068831217,0.0009009985,0.0028112677],"category_scores_gemma":[0.00039491314,0.00020052103,0.00022735333,0.0008511977,0.00038080494,0.00027453213,0.00071289664,0.00032708124,0.0010552729],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00088057166,0.00059544656,0.71329004,0.00034207007,0.000121906385,0.02011892,0.00097031245,0.0012900962,0.18044677,0.002419461,0.011875186,0.06764932],"study_design_scores_gemma":[0.00007159012,0.00027494616,0.9488304,0.00004582034,0.000045153774,0.016984519,0.00038886236,0.003100123,0.009787552,0.0006646414,0.019758007,0.000048324484],"about_ca_topic_score_codex":0.0038677135,"about_ca_topic_score_gemma":0.0040501007,"teacher_disagreement_score":0.0038677135,"about_ca_system_score_codex":0.00046056637,"about_ca_system_score_gemma":0.00025822275,"threshold_uncertainty_score":0.0094046},"labels":[],"label_agreement":null},{"id":"W2016772770","doi":"10.1088/0004-637x/766/2/116","title":"STUDIES OF VARIABILITY IN PROTO-PLANETARY NEBULAE. II. LIGHT AND VELOCITY CURVE ANALYSES OF IRAS 22272+5435 AND 22223+4327","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Light curve; Astrophysics; Cepheid variable; Physics; Amplitude; Radial velocity; Stars; Phase (matter); Optics","score_opus":0.026498645281684774,"score_gpt":0.2800001466042708,"score_spread":0.25350150132258603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016772770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984616,0.00016014533,0.00021005522,0.000012819293,0.0000025637069,0.000005959774,0.00029862922,0.000012762133,0.00083546585],"genre_scores_gemma":[0.9976267,0.00012456723,0.0006317159,0.000017613822,0.000007262474,0.000010729515,0.0010151825,0.000009605198,0.00055652665],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987507,0.000011881097,0.000007045979,0.000040864783,0.000035997244,0.000029170144],"domain_scores_gemma":[0.9994338,0.00007069771,0.00022554674,0.000041475352,0.00014030571,0.00008812521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020806177,0.00022520301,0.00017302897,0.001371991,0.0003903409,0.00034455856,0.00028649767,0.00019219762,0.000666292],"category_scores_gemma":[0.0005989464,0.00010259742,0.0001977282,0.0012708083,0.00017615057,0.0002088821,0.00023386028,0.00024458865,0.00025297928],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000100150355,0.00011534977,0.934238,0.00006899421,0.00006631419,0.0001856712,0.00064064935,0.00059967506,0.043281395,0.0002748668,0.000446055,0.019982938],"study_design_scores_gemma":[9.697112e-7,0.000021326568,0.99769115,0.0000019550148,0.0000045215756,0.000070285285,0.000054037813,0.00018568299,0.000978973,0.00001996364,0.0009682886,0.0000029703654],"about_ca_topic_score_codex":0.00927411,"about_ca_topic_score_gemma":0.022547226,"teacher_disagreement_score":0.00927411,"about_ca_system_score_codex":0.00044462044,"about_ca_system_score_gemma":0.00020307736,"threshold_uncertainty_score":0.018440306},"labels":[],"label_agreement":null},{"id":"W2016781916","doi":"10.1088/0004-637x/692/1/l62","title":"CONSTRAINING THE SPIN-DOWN OF THE NEARBY ISOLATED NEUTRON STAR RX J2143.0+0654","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Neutron star; Astrophysics; Population; Magnetic field; Spectral line; Spin (aerodynamics); Absorption (acoustics); Neutron; Field (mathematics); Dipole; Astronomy; Nuclear physics; Optics; Quantum mechanics","score_opus":0.011685078174709509,"score_gpt":0.23488546851329498,"score_spread":0.22320039033858546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016781916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990202,0.000071324466,0.00018331487,0.000016052129,0.0000033485373,0.0000023345945,0.00006721318,0.000010651102,0.00062544894],"genre_scores_gemma":[0.99913543,0.00004463907,0.00043026093,0.000013359754,0.000007078996,0.0000028752395,0.00020409861,0.00000556825,0.0001567162],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998604,0.000024612655,0.000014059422,0.00005098431,0.00002305891,0.000026876965],"domain_scores_gemma":[0.99926895,0.00008774507,0.00034799794,0.00008778927,0.00006663552,0.0001409606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004983948,0.00039993395,0.00039554818,0.0009276263,0.00043670577,0.00060107955,0.00035006195,0.0004646447,0.00093946396],"category_scores_gemma":[0.0011594495,0.00025209418,0.0002748485,0.00041263702,0.0002909742,0.0002623341,0.00052654056,0.0003453887,0.0004943586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004502625,0.000067642926,0.8672729,0.00004976165,0.00010854214,0.00037225863,0.00022647379,0.0011499994,0.12068539,0.0005597953,0.00027617678,0.00878079],"study_design_scores_gemma":[0.000039096907,0.00017980907,0.9849194,0.000017212675,0.00009119888,0.0006282163,0.00013457629,0.0043317378,0.00830721,0.00032478926,0.0010107777,0.000015907284],"about_ca_topic_score_codex":0.0016499261,"about_ca_topic_score_gemma":0.0028954302,"teacher_disagreement_score":0.0016499261,"about_ca_system_score_codex":0.00029382433,"about_ca_system_score_gemma":0.0001183862,"threshold_uncertainty_score":0.0032806396},"labels":[],"label_agreement":null},{"id":"W2016849810","doi":"10.1088/0004-637x/731/1/70","title":"A<i>CHANDRA</i>OBSERVATION OF SUPERNOVA REMNANT G350.1–0.3 AND ITS CENTRAL COMPACT OBJECT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Ejecta; Physics; Astrophysics; Supernova remnant; Supernova; Astronomy; Spitzer Space Telescope; Infrared; Telescope","score_opus":0.02542790368767052,"score_gpt":0.22095830027310193,"score_spread":0.19553039658543142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016849810","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995355,0.00033561813,0.00037964963,0.00005015303,0.000013081352,0.000025346508,0.0013115542,0.00019908663,0.0023305272],"genre_scores_gemma":[0.99206686,0.00017771151,0.0030546864,0.00007992459,0.000033196782,0.000013974985,0.0036382095,0.000033680182,0.00090178114],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999267,0.0000030653885,0.000003282612,0.000018967588,0.000023106208,0.000024854748],"domain_scores_gemma":[0.999754,0.000010559378,0.000058931102,0.000030474896,0.000026271327,0.00011988445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013319198,0.00028806104,0.0002535767,0.0011083131,0.00043691605,0.00036018892,0.0003319818,0.00024036791,0.0009212418],"category_scores_gemma":[0.0001594658,0.00016614427,0.00033204127,0.00063184986,0.00018746396,0.00022994478,0.00045495515,0.00029650755,0.00024969774],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002176503,0.00041056576,0.3956803,0.0003435052,0.00046689514,0.0077181244,0.000993464,0.0011397129,0.5361778,0.0009235901,0.0057236245,0.048245873],"study_design_scores_gemma":[0.00002927234,0.00025878008,0.98243225,0.000015486552,0.000075213626,0.002867653,0.00010562759,0.0006360719,0.007976581,0.00012816605,0.005453258,0.0000216032],"about_ca_topic_score_codex":0.0063196113,"about_ca_topic_score_gemma":0.014365076,"teacher_disagreement_score":0.0063196113,"about_ca_system_score_codex":0.0002374088,"about_ca_system_score_gemma":0.00023542541,"threshold_uncertainty_score":0.012565672},"labels":[],"label_agreement":null},{"id":"W2016875427","doi":"10.1088/0004-637x/791/1/46","title":"HOT ELECTROMAGNETIC OUTFLOWS. III. DISPLACED FIREBALL IN A STRONG MAGNETIC FIELD","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Lorentz factor; Compton scattering; Gamma-ray burst; Baryon; Luminosity; Photosphere; Photon; Magnetic field; Scattering","score_opus":0.005493184197818829,"score_gpt":0.21293133085648877,"score_spread":0.20743814665866994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016875427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949529,0.00014732647,0.001362073,0.00005141069,0.000011194317,0.0000119795395,0.00006921304,0.000037288813,0.0033566768],"genre_scores_gemma":[0.99894124,0.00004728168,0.00036886273,0.000019182393,0.000009423162,0.0000053969748,0.00006587935,0.000010648117,0.00053211936],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992526,0.000015091975,0.0000041787735,0.000011311778,0.000013172684,0.000030914907],"domain_scores_gemma":[0.99972504,0.00005709977,0.00008194155,0.000022239752,0.00003057354,0.00008297421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002565276,0.00037327004,0.00037716696,0.00041892522,0.00041440045,0.0010416559,0.0006269502,0.00050546473,0.0011231835],"category_scores_gemma":[0.0010061149,0.00022406083,0.0005546826,0.00023784245,0.00071984815,0.000440797,0.0005649081,0.00046894696,0.00014597848],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013117159,0.0002744514,0.087968886,0.00031165447,0.00030384664,0.0034145934,0.00028224758,0.78125507,0.08691699,0.03010528,0.0006207623,0.007234584],"study_design_scores_gemma":[0.0001992454,0.0002071765,0.033355586,0.000023764447,0.000047449932,0.00041596818,0.00013946032,0.9538318,0.008420329,0.0028044202,0.0005239504,0.000030969743],"about_ca_topic_score_codex":0.0030007716,"about_ca_topic_score_gemma":0.0012345844,"teacher_disagreement_score":0.0030007716,"about_ca_system_score_codex":0.000767694,"about_ca_system_score_gemma":0.00021635089,"threshold_uncertainty_score":0.0059666038},"labels":[],"label_agreement":null},{"id":"W2016921116","doi":"10.1088/0004-637x/796/2/89","title":"TRACING RAM-PRESSURE STRIPPING WITH WARM MOLECULAR HYDROGEN EMISSION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Galaxy; Star formation; Intracluster medium; Spectrograph; Extinction (optical mineralogy); Galaxy formation and evolution; Spiral galaxy; Line (geometry)","score_opus":0.00445654851673236,"score_gpt":0.1956210495018274,"score_spread":0.19116450098509505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016921116","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99946886,0.000018422697,0.00023671899,0.0000046203545,5.291787e-7,0.000002402203,0.00003475403,0.000023378325,0.00021035639],"genre_scores_gemma":[0.99905366,0.000011399841,0.00069083885,0.0000049608716,0.0000019563781,0.000002041292,0.00012673499,0.000003598131,0.000104776416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990773,0.000009264752,0.000002235938,0.00002140667,0.000020782296,0.000038620998],"domain_scores_gemma":[0.99967337,0.00005473501,0.00010702143,0.000035505072,0.000038493083,0.00009092862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015550017,0.00024092043,0.00019497071,0.001006845,0.00026978148,0.0003462013,0.00037762028,0.00025543958,0.00034018603],"category_scores_gemma":[0.00041094766,0.00015835013,0.00017726938,0.0005050934,0.00019809013,0.0001761378,0.0003926529,0.00020840763,0.000116293],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028648693,0.0001582205,0.88035107,0.000029320036,0.00009086636,0.0013045507,0.0008698949,0.0021974253,0.09907839,0.00016607351,0.00024468984,0.015222957],"study_design_scores_gemma":[0.0000063917737,0.00009759158,0.9847548,0.00000300029,0.000021162701,0.00034134812,0.00022670219,0.007222471,0.0069204657,0.000073012256,0.0003238656,0.0000091572865],"about_ca_topic_score_codex":0.0056358124,"about_ca_topic_score_gemma":0.007287018,"teacher_disagreement_score":0.0056358124,"about_ca_system_score_codex":0.00033465135,"about_ca_system_score_gemma":0.0000913654,"threshold_uncertainty_score":0.011205971},"labels":[],"label_agreement":null},{"id":"W2016962043","doi":"10.1088/0004-637x/754/2/96","title":"<i>CHANDRA</i>AND<i>XMM-NEWTON</i>STUDIES OF THE SUPERNOVA REMNANT G292.2-0.5 ASSOCIATED WITH THE PULSAR J1119-6127","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Manitoba","funders":"","keywords":"Supernova remnant; Ejecta; Pulsar; Near-Earth supernova; Spectral line; Ionization; Nucleosynthesis","score_opus":0.020736236187960295,"score_gpt":0.3044147399447424,"score_spread":0.2836785037567821,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2016962043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971091,0.0004597849,0.00027747042,0.000014271862,0.0000035973487,0.000009538641,0.0001777415,0.000019992298,0.0019284313],"genre_scores_gemma":[0.9962894,0.00041845255,0.0015452115,0.000032974574,0.0000124253975,0.000008121891,0.0010324346,0.000016042255,0.00064503256],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992096,0.000006278753,0.000006215969,0.00002228709,0.00002353503,0.000020744788],"domain_scores_gemma":[0.99977106,0.000015097061,0.00009924202,0.000026764123,0.000036648777,0.0000510707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017945575,0.00028921245,0.00020436988,0.00096785004,0.00041079216,0.00039337136,0.0002952956,0.00014941793,0.0005528263],"category_scores_gemma":[0.00021763549,0.00018806926,0.00029297787,0.00051572686,0.0002961163,0.00021553514,0.0004921082,0.00023775766,0.00023173369],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005029763,0.00020946946,0.47310442,0.00024376987,0.000203529,0.003138116,0.0009657085,0.0011451498,0.5043663,0.0007263867,0.0005191655,0.014875015],"study_design_scores_gemma":[0.000013002028,0.00015745386,0.9810167,0.0000136369545,0.000040880655,0.0025816252,0.00025838555,0.0004835645,0.012434797,0.00009297684,0.0028926746,0.000014355744],"about_ca_topic_score_codex":0.0033678992,"about_ca_topic_score_gemma":0.0078890165,"teacher_disagreement_score":0.0033678992,"about_ca_system_score_codex":0.00024177827,"about_ca_system_score_gemma":0.00016959467,"threshold_uncertainty_score":0.006696582},"labels":[],"label_agreement":null},{"id":"W2017025447","doi":"10.1086/340500","title":"Globular Clusters at High Redshift","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Globular cluster; Redshift; Astronomy; Galaxy; Population; Sky; Elliptical galaxy","score_opus":0.007758276628292007,"score_gpt":0.19304712206850583,"score_spread":0.18528884544021382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017025447","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6570319,0.009921428,0.017284114,0.0059876335,0.00047271766,0.00010622493,0.0045748944,0.0018205728,0.3028006],"genre_scores_gemma":[0.9694258,0.0017002911,0.0029255436,0.0007989482,0.0002478248,0.000023131874,0.0014626943,0.00007205155,0.023343861],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99966204,0.000022211605,0.000005966132,0.00008172131,0.0001307185,0.00009735348],"domain_scores_gemma":[0.999308,0.0000739266,0.00012585706,0.00012626882,0.00014583615,0.00022025369],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004304662,0.00021221329,0.0003367887,0.0011483978,0.0013187539,0.0018163363,0.00029635438,0.00062149647,0.010761974],"category_scores_gemma":[0.0014792496,0.00016128969,0.0001399931,0.0016733977,0.0005671903,0.0010156058,0.0013109259,0.00064011407,0.0031789353],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017623363,0.00006133716,0.25887355,0.0003131468,0.00009448691,0.00086998416,0.0033781107,0.0022185727,0.012263494,0.50447124,0.07136513,0.14591472],"study_design_scores_gemma":[0.000039968145,0.00005213838,0.6133329,0.0000848613,0.00006259034,0.0013035273,0.0009619123,0.0016519488,0.0023470689,0.14503178,0.2350657,0.0000655266],"about_ca_topic_score_codex":0.0066640344,"about_ca_topic_score_gemma":0.0055916347,"teacher_disagreement_score":0.010761974,"about_ca_system_score_codex":0.0010974319,"about_ca_system_score_gemma":0.00033407405,"threshold_uncertainty_score":0.036002398},"labels":[],"label_agreement":null},{"id":"W2017035786","doi":"10.1086/501492","title":"Surface Temperature and Synthetic Spectral Energy Distributions for Rotationally Deformed Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Effective temperature; Astrophysics; Surface gravity; Stars; Spectral energy distribution; Luminosity; Spectral line; Rotation (mathematics); Geometry; Astronomy; Galaxy","score_opus":0.005271253571657865,"score_gpt":0.204211586803618,"score_spread":0.19894033323196014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017035786","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98239547,0.000028440201,0.015064631,0.000029937713,0.000008922791,0.000010577691,0.00067176356,0.00034005128,0.0014502946],"genre_scores_gemma":[0.99269754,0.000015762333,0.005935213,0.000007773316,0.0000031766767,0.0000084503845,0.0010446742,0.00009937496,0.00018808608],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999018,0.000014450973,0.0000060829757,0.00003535517,0.000027083175,0.00001526148],"domain_scores_gemma":[0.99961627,0.000084843756,0.000048168145,0.000087431275,0.00012079425,0.00004248826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025748005,0.00022890464,0.0001840392,0.00063619454,0.00020854519,0.0004508336,0.00031377585,0.00033919327,0.00077937456],"category_scores_gemma":[0.0009929466,0.00019168611,0.0005234617,0.0005896717,0.00025696136,0.00032405503,0.00021141092,0.00030084283,0.00028600154],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005047733,0.00011854189,0.11419388,0.000057031608,0.00009729533,0.00029897603,0.0002566541,0.7895781,0.073076986,0.0059051444,0.0008731654,0.015039356],"study_design_scores_gemma":[0.000043655124,0.00006496603,0.06916298,0.0000034943002,0.000017600256,0.00017790351,0.000058799156,0.9121804,0.015528612,0.0019477585,0.00078484445,0.00002905217],"about_ca_topic_score_codex":0.0022642391,"about_ca_topic_score_gemma":0.0017053101,"teacher_disagreement_score":0.0022642391,"about_ca_system_score_codex":0.0005775754,"about_ca_system_score_gemma":0.00015458844,"threshold_uncertainty_score":0.0045021772},"labels":[],"label_agreement":null},{"id":"W2017046269","doi":"10.1088/0004-637x/756/2/149","title":"<i>SUZAKU</i>OBSERVATIONS OF THE NON-THERMAL SUPERNOVA REMNANT HESS J1731–347","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Supernova remnant; Supernova; Shell (structure); Thermal emission; Absorption (acoustics); Photon; Electron; Thermal; Spectral index; Curvature; Astronomy; Optics; Spectral line; Materials science; Geometry; Nuclear physics","score_opus":0.015525557236389759,"score_gpt":0.2211990991943022,"score_spread":0.20567354195791243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017046269","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26291224,0.012684791,0.0057249176,0.024448583,0.04014193,0.00042850117,0.38923892,0.015919399,0.24850069],"genre_scores_gemma":[0.29795074,0.007673367,0.020417517,0.004948907,0.015231468,0.00021809868,0.51095057,0.003290848,0.13931847],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99987745,0.0000070113947,0.00001394014,0.000018779721,0.00005656347,0.000026228832],"domain_scores_gemma":[0.99918896,0.00008805541,0.00020422132,0.00014663639,0.00019767607,0.00017428453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032272958,0.00071809645,0.00036680928,0.004476945,0.00085861626,0.0012693446,0.00069141795,0.00065231055,0.047305275],"category_scores_gemma":[0.00068659923,0.00042659786,0.0007357719,0.0037695407,0.00041327492,0.0009969453,0.0010675697,0.00088855095,0.015896184],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046179027,0.00008310175,0.02835572,0.0008062484,0.0002500514,0.0012560263,0.00020789263,0.0003598157,0.019243639,0.002205769,0.90636164,0.040408418],"study_design_scores_gemma":[0.000055766213,0.00008335905,0.42834663,0.00016284591,0.00009586446,0.00089320785,0.0001636444,0.00034782544,0.004374966,0.0009900426,0.56440157,0.00008427027],"about_ca_topic_score_codex":0.01111362,"about_ca_topic_score_gemma":0.047025867,"teacher_disagreement_score":0.047305275,"about_ca_system_score_codex":0.00058016,"about_ca_system_score_gemma":0.00052062195,"threshold_uncertainty_score":0.15825194},"labels":[],"label_agreement":null},{"id":"W2017260657","doi":"10.1086/521383","title":"A Dark Core in Abell 520","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":169,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Astrophysics; Physics; Dark matter; Galaxy cluster; Abell 2744; Galaxy; Astronomy; Ram pressure; Dark galaxy; Galaxy group; Star formation","score_opus":0.009677903814985192,"score_gpt":0.22909310722741894,"score_spread":0.21941520341243376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017260657","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99384993,0.00010551706,0.00007105231,0.000081732986,0.0000059954295,0.000004578301,0.00054657616,0.000028092098,0.005306561],"genre_scores_gemma":[0.9974693,0.000024883679,0.0001331664,0.00004550882,0.0000072941984,0.000001920907,0.0010664228,0.0000073899705,0.0012442749],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999273,0.000004731984,0.000002162134,0.000018781158,0.000011822794,0.00003521276],"domain_scores_gemma":[0.99984276,0.000009061309,0.000036470716,0.00001052086,0.000012430734,0.00008878929],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007775624,0.00016703412,0.00019653089,0.0006303807,0.00091321603,0.00059182936,0.00014553261,0.00030222101,0.0026438863],"category_scores_gemma":[0.00020875488,0.00012239312,0.000091791386,0.00041862723,0.00024239226,0.00019967507,0.00060437,0.0002200549,0.0007124586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026458916,0.00047380553,0.727689,0.00018570086,0.0001043943,0.011723483,0.0043247673,0.0015443896,0.1857523,0.016627846,0.019877883,0.029050518],"study_design_scores_gemma":[0.00001641201,0.00007891768,0.9905928,0.000013138791,0.0000106565885,0.0005555322,0.00043641706,0.0004825114,0.0017654087,0.0005253995,0.005508391,0.000014342305],"about_ca_topic_score_codex":0.042133283,"about_ca_topic_score_gemma":0.06005923,"teacher_disagreement_score":0.042133283,"about_ca_system_score_codex":0.0010480183,"about_ca_system_score_gemma":0.00033208815,"threshold_uncertainty_score":0.08377606},"labels":[],"label_agreement":null},{"id":"W2017450811","doi":"10.1088/0004-637x/766/2/136","title":"STELLAR ENCOUNTER RATE IN GALACTIC GLOBULAR CLUSTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Millisecond pulsar; Surface brightness; Star cluster; Luminosity; Stellar density; Cluster (spacecraft); Astronomy; Brightness; Pulsar; Stellar evolution; Stars; Galaxy","score_opus":0.007930725733843064,"score_gpt":0.21297540558598824,"score_spread":0.20504467985214517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017450811","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99836594,0.00006811653,0.0011129526,0.000003883101,5.217413e-7,0.000002915979,0.00007909164,0.00001981,0.0003468297],"genre_scores_gemma":[0.99924326,0.000034036755,0.00045605583,0.0000015721422,5.2785873e-7,0.0000022423162,0.0001764419,0.0000061654614,0.00007966135],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99970055,0.00007301656,0.00002462001,0.00010090123,0.000070351256,0.00003057474],"domain_scores_gemma":[0.9959092,0.0021680114,0.0008603206,0.00047938217,0.0004165604,0.00016646682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009622621,0.0001912516,0.00022972871,0.0014400923,0.0002899244,0.00062430126,0.00047074788,0.00035849493,0.0004066068],"category_scores_gemma":[0.007775053,0.00018893558,0.00020470258,0.0010662981,0.00049500697,0.00043325365,0.00052442885,0.00013851708,0.00017847454],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103117076,0.000010579881,0.94386727,0.000011542822,0.000037527327,0.000042137133,0.00020089585,0.049995564,0.0011280795,0.0006537742,0.00007362912,0.0038759697],"study_design_scores_gemma":[0.000015622429,0.00011483758,0.82383066,0.000017006087,0.000047094247,0.0003815662,0.00035702236,0.16446207,0.008106801,0.0019632927,0.0006593162,0.000044761466],"about_ca_topic_score_codex":0.008865118,"about_ca_topic_score_gemma":0.004437208,"teacher_disagreement_score":0.008865118,"about_ca_system_score_codex":0.0009446816,"about_ca_system_score_gemma":0.00020782185,"threshold_uncertainty_score":0.01762706},"labels":[],"label_agreement":null},{"id":"W2017540369","doi":"10.1086/527028","title":"The Initial‐Final Mass Relation: Direct Constraints at the Low‐Mass End","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":319,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"White dwarf; Stars; Balmer series; Low Mass; Open cluster; Brown dwarf; Spectral line; Stellar mass; Mass spectrum","score_opus":0.022472364442165424,"score_gpt":0.23987889618560462,"score_spread":0.2174065317434392,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017540369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9812571,0.0006120533,0.011468107,0.000105708,0.000008479103,0.000011665128,0.00041035825,0.00011508677,0.0060114088],"genre_scores_gemma":[0.99716127,0.00006106759,0.0019276782,0.000034279765,0.000010426848,0.000007043535,0.0003690033,0.00002423187,0.0004049712],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974877,0.000025256446,0.000014676087,0.000099934434,0.000043977798,0.000067434004],"domain_scores_gemma":[0.99743015,0.0009864307,0.0006357864,0.0003172923,0.00026629958,0.00036398837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006559223,0.00044447763,0.0004296213,0.0010983042,0.00093626225,0.0017710346,0.0008033579,0.00071309233,0.0025146813],"category_scores_gemma":[0.0025112533,0.00027449313,0.00031865752,0.0005429814,0.00078728324,0.0009898315,0.00110838,0.00070910895,0.0008837222],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026204158,0.00006733071,0.94007635,0.00007529034,0.000050249884,0.00026433013,0.0006667397,0.0019526342,0.032159694,0.0067327893,0.00044473694,0.017247735],"study_design_scores_gemma":[0.00001536393,0.00010658865,0.9703325,0.000029215458,0.000035678764,0.00029637764,0.00028417513,0.009619391,0.012033377,0.004724922,0.0024978763,0.000024464916],"about_ca_topic_score_codex":0.0042302334,"about_ca_topic_score_gemma":0.0058760894,"teacher_disagreement_score":0.0042302334,"about_ca_system_score_codex":0.0005681742,"about_ca_system_score_gemma":0.00027278613,"threshold_uncertainty_score":0.00841248},"labels":[],"label_agreement":null},{"id":"W2017569741","doi":"10.1086/527030","title":"Mid‐Infrared Spectral Diagnosis of Submillimeter Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":378,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Canadian Space Agency; National Aeronautics and Space Administration; California Institute of Technology; Ames Research Center","keywords":"Physics; Astrophysics; Star formation; Redshift; Galaxy; Luminous infrared galaxy; Infrared; Astronomy; Luminosity; Photometry (optics); Stars","score_opus":0.01063597717670465,"score_gpt":0.2050210740140036,"score_spread":0.19438509683729896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017569741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99807715,0.000058864698,0.00026692633,0.000011840069,0.0000015903096,0.000004037153,0.00022591263,0.000040873394,0.0013128216],"genre_scores_gemma":[0.9985947,0.000020179465,0.000619508,0.000017616978,0.0000035971227,0.000005261548,0.00047291722,0.000004559587,0.00026160915],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989593,0.000008592199,0.000008170251,0.000023305265,0.0000186163,0.00004530654],"domain_scores_gemma":[0.9994362,0.00006195167,0.0002279819,0.000046045727,0.000067324196,0.00016046666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022746024,0.0002496775,0.00013472684,0.0018501891,0.00022897143,0.0004103628,0.00022155937,0.00017974601,0.0016068254],"category_scores_gemma":[0.00046157662,0.00012705782,0.00020630028,0.0005468787,0.00016938524,0.00021817986,0.0005046213,0.00018460935,0.00046632593],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006115969,0.000019383393,0.97940534,0.000009475367,0.000012264306,0.00007803019,0.00016413043,0.00018509342,0.012662406,0.00012103155,0.00015880857,0.007122902],"study_design_scores_gemma":[9.211694e-7,0.000015071071,0.99911755,0.0000017947993,0.0000023735859,0.0000663193,0.00005652167,0.00019288746,0.00033687524,0.000030048019,0.00017833833,0.0000012507082],"about_ca_topic_score_codex":0.0020190696,"about_ca_topic_score_gemma":0.0037591872,"teacher_disagreement_score":0.0020190696,"about_ca_system_score_codex":0.00021662976,"about_ca_system_score_gemma":0.000080184975,"threshold_uncertainty_score":0.0053753257},"labels":[],"label_agreement":null},{"id":"W2017576685","doi":"10.1088/0004-637x/780/1/69","title":"SUPERMASSIVE BLACK HOLES AND THEIR HOST GALAXIES. I. BULGE LUMINOSITIES FROM DEDICATED NEAR-INFRARED DATA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Bulge; Supermassive black hole; Galaxy; Surface brightness; Brightness; Quasar; Scaling","score_opus":0.011281019376089744,"score_gpt":0.2034057205963293,"score_spread":0.19212470122023956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017576685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977385,0.00030257856,0.00074464496,0.000007760428,0.0000017691784,0.000007785151,0.0007078584,0.000020944588,0.00046811733],"genre_scores_gemma":[0.99805886,0.00008632496,0.0006633184,0.000005636679,0.000004284693,0.0000059660806,0.0010558232,0.0000047690605,0.00011507146],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998535,0.000020733896,0.000015238607,0.000054408483,0.00002809328,0.000027963852],"domain_scores_gemma":[0.9993754,0.000110882684,0.00030906763,0.00008554976,0.000033400385,0.000085770975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036586405,0.00031128642,0.00022353993,0.0017000209,0.0001630253,0.00040554575,0.00028764005,0.0002137151,0.0008971428],"category_scores_gemma":[0.000972297,0.00017924354,0.00022400911,0.0006637369,0.00027294562,0.0004936742,0.0005331864,0.00021894215,0.00033809093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001246167,0.000014774479,0.9865443,0.000031573913,0.000034808563,0.000075567856,0.00021374035,0.0006322478,0.0053782947,0.00016864901,0.0000964156,0.0066851284],"study_design_scores_gemma":[0.0000017867566,0.00001948885,0.9982476,0.0000039618253,0.000009352538,0.000060325732,0.000048261594,0.00075435796,0.00048015002,0.00007963551,0.00029302458,0.0000021341018],"about_ca_topic_score_codex":0.004204801,"about_ca_topic_score_gemma":0.007231333,"teacher_disagreement_score":0.004204801,"about_ca_system_score_codex":0.00021208607,"about_ca_system_score_gemma":0.00006396087,"threshold_uncertainty_score":0.008360684},"labels":[],"label_agreement":null},{"id":"W2017627447","doi":"10.1086/587165","title":"The Outer Scale of Turbulence in the Magnetoionized Galactic Interstellar Medium","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":238,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Spiral galaxy; Interstellar medium; Galaxy; Supernova; Amplitude; Turbulence; Rotation (mathematics); Galactic plane; Spectral density; Astronomy; Geometry; Mechanics; Optics","score_opus":0.01056770306457157,"score_gpt":0.22602841877799085,"score_spread":0.21546071571341927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017627447","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99450594,0.00020617605,0.0036067285,0.000059692513,0.000010792987,0.0000040256664,0.000048651265,0.00003720125,0.001520793],"genre_scores_gemma":[0.99954104,0.00005400126,0.00026205147,0.0000027246442,0.0000064590895,0.0000015069057,0.000035931964,0.0000037817836,0.000092625975],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999497,0.000007865527,0.000002352037,0.000009551904,0.000008695457,0.00002181662],"domain_scores_gemma":[0.99966717,0.00010872092,0.00010351018,0.00001542801,0.000029343468,0.00007577916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109791836,0.00028294086,0.00013423187,0.0005856873,0.00027720543,0.0007388347,0.000113932205,0.0001249647,0.0002731893],"category_scores_gemma":[0.00065896334,0.00012065355,0.0001752429,0.00020760993,0.0003980478,0.00047842631,0.00047070798,0.00024373754,0.000056342764],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013115968,0.00028058808,0.40099153,0.000115967654,0.00025195017,0.0029503584,0.00083294546,0.19736253,0.29585183,0.06998507,0.0010208274,0.029044865],"study_design_scores_gemma":[0.000037764417,0.00018902445,0.52111876,0.000018446748,0.00007721881,0.00044248725,0.00025758785,0.44454187,0.015240139,0.01669584,0.0012830704,0.000097785814],"about_ca_topic_score_codex":0.0015888702,"about_ca_topic_score_gemma":0.0010094426,"teacher_disagreement_score":0.0015888702,"about_ca_system_score_codex":0.00034057657,"about_ca_system_score_gemma":0.0001305123,"threshold_uncertainty_score":0.0031592846},"labels":[],"label_agreement":null},{"id":"W2017667374","doi":"10.1086/309203","title":"The 35 Day Evolution of the Hercules X‐1 Pulse Profile: Evidence for a Resolved Inner Disk Occultation of the Neutron Star","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Neutron star; Pulsar; Occultation; Accretion (finance); Pulse (music); Millisecond pulsar; Accretion disc","score_opus":0.019594200929748208,"score_gpt":0.2584558670608353,"score_spread":0.23886166613108709,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017667374","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955428,0.0009928215,0.0005638987,0.00006898151,0.000012687769,0.000009809381,0.0004472949,0.00006967156,0.002292077],"genre_scores_gemma":[0.99831057,0.00026561657,0.00038108518,0.000031200412,0.000017651331,0.000006906878,0.0005484359,0.000013015648,0.0004254754],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999727,0.0000026349005,0.000001446636,0.000010282392,0.000007716079,0.0000052215137],"domain_scores_gemma":[0.9998085,0.000028735223,0.00008162361,0.000019934816,0.0000302378,0.00003096594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010278142,0.00013235031,0.00013442425,0.00054654205,0.00016565279,0.0003166439,0.00017374962,0.00024973444,0.00065621175],"category_scores_gemma":[0.00023780708,0.000101745805,0.00009778046,0.00046193795,0.00015192188,0.00012763607,0.00021774384,0.00024425887,0.00020375407],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012694467,0.00011247232,0.45286688,0.00032703837,0.00013001084,0.0031458444,0.00085965125,0.0013158034,0.4563759,0.0010908575,0.002541803,0.07996421],"study_design_scores_gemma":[0.000004554024,0.000054067048,0.9932114,0.000008375509,0.0000109162365,0.0005215651,0.000032385873,0.00037090806,0.0044322615,0.000078449375,0.0012702614,0.0000048253123],"about_ca_topic_score_codex":0.0009222606,"about_ca_topic_score_gemma":0.0010663942,"teacher_disagreement_score":0.0009222606,"about_ca_system_score_codex":0.00021251987,"about_ca_system_score_gemma":0.00007396006,"threshold_uncertainty_score":0.002195239},"labels":[],"label_agreement":null},{"id":"W2017690860","doi":"10.1088/0004-637x/797/2/76","title":"CARMA LARGE AREA STAR FORMATION SURVEY: STRUCTURE AND KINEMATICS OF DENSE GAS IN SERPENS MAIN","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Serpens; Velocity dispersion; Line (geometry); Kinematics; Star formation; Molecular cloud; Dendrogram; Galaxy","score_opus":0.010031125425351095,"score_gpt":0.2291020998839244,"score_spread":0.21907097445857332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017690860","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990351,0.00009897272,0.00004069199,0.000009659307,0.0000017503435,0.00000432845,0.0002459221,0.000014624633,0.0005489188],"genre_scores_gemma":[0.9988708,0.00009458289,0.00020979048,0.000008236785,0.0000061297283,0.000004318165,0.00057425717,0.000003858773,0.00022808404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999188,0.00000939269,0.00000387057,0.000022036655,0.00002099272,0.000024928757],"domain_scores_gemma":[0.9998511,0.000014008017,0.000055690165,0.000016150309,0.000016034499,0.00004694925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012033839,0.00024178589,0.00016052899,0.0012273215,0.00020570101,0.0003068972,0.00028890543,0.00016137151,0.0010739046],"category_scores_gemma":[0.00026456505,0.00011898931,0.00013883099,0.00046058724,0.00018777594,0.0001461325,0.00034774357,0.00009734896,0.00023356148],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028255713,0.00007558092,0.95309275,0.00007431617,0.00007984542,0.00083254254,0.00074625894,0.0011094683,0.026186738,0.00017783779,0.0009927555,0.01634935],"study_design_scores_gemma":[0.000007315931,0.00003356021,0.99709785,0.000005667316,0.000010532409,0.00012234616,0.00007896083,0.0005571352,0.00075418176,0.000015102814,0.0013151771,0.0000022179775],"about_ca_topic_score_codex":0.012884788,"about_ca_topic_score_gemma":0.025329173,"teacher_disagreement_score":0.012884788,"about_ca_system_score_codex":0.00043266654,"about_ca_system_score_gemma":0.0002537281,"threshold_uncertainty_score":0.025619566},"labels":[],"label_agreement":null},{"id":"W2017701380","doi":"10.1086/499582","title":"Formation of Minigalaxies in Defunct Cosmological H<scp>ii</scp>Regions","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Redshift; Star formation; Galaxy formation and evolution; Galaxy; Virial theorem; Universe; Quasar; Astronomy","score_opus":0.009469652584089282,"score_gpt":0.2044919124201752,"score_spread":0.19502225983608593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017701380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982855,0.000045475874,0.00063140824,0.000047187685,0.0000041640264,0.000011660406,0.00010962346,0.000027654258,0.00083729083],"genre_scores_gemma":[0.9987225,0.000042632753,0.0006596828,0.000037673686,0.0000050266513,0.000014427667,0.00015780253,0.000013302854,0.00034709423],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993026,0.000014581546,0.0000024115245,0.000012689416,0.0000071167665,0.00003292885],"domain_scores_gemma":[0.99953735,0.000089999405,0.00012186003,0.00003199316,0.000024095874,0.00019471135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033001738,0.0003454071,0.00036962028,0.00039619562,0.0005807633,0.0008999861,0.00081019936,0.00063331675,0.0015836458],"category_scores_gemma":[0.0010396101,0.0004491373,0.0005826559,0.00025206315,0.00084240746,0.00051295344,0.00095712475,0.0005697756,0.000101056095],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042067657,0.00021608242,0.08848307,0.00006609162,0.00018044068,0.00077662326,0.00040698415,0.8885564,0.007154855,0.0103410175,0.0009398446,0.0024580231],"study_design_scores_gemma":[0.00021839308,0.00017454343,0.047847863,0.000011321081,0.00005342478,0.00013015413,0.00020457675,0.94645655,0.0012369596,0.0031545085,0.0004880371,0.000023671766],"about_ca_topic_score_codex":0.018094702,"about_ca_topic_score_gemma":0.010502141,"teacher_disagreement_score":0.018094702,"about_ca_system_score_codex":0.0011472015,"about_ca_system_score_gemma":0.00048488096,"threshold_uncertainty_score":0.035978734},"labels":[],"label_agreement":null},{"id":"W2017776000","doi":"10.1086/506014","title":"A Study of H<sub>2</sub>Emission in the Bipolar Proto–Planetary Nebula IRAS 17150−3224","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Planetary nebula; Line (geometry); Emission spectrum; Spectral line; Nebula; Astronomy; Stars","score_opus":0.009294439721585177,"score_gpt":0.2280639847563765,"score_spread":0.21876954503479132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017776000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99766433,0.0004945295,0.00016790375,0.000019294397,0.0000039797865,0.0000055562086,0.00007100927,0.000009177253,0.0015642428],"genre_scores_gemma":[0.997801,0.00037588438,0.00048420244,0.000051708827,0.000016545711,0.0000067171977,0.0003663748,0.0000053666135,0.0008921874],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999739,0.0000023574162,5.768289e-7,0.0000065120275,0.000007363291,0.000009202157],"domain_scores_gemma":[0.99995875,0.0000061934215,0.000012210822,0.000003672569,0.0000057588163,0.000013503084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000066066066,0.00017843525,0.00009067166,0.0003547362,0.00028879085,0.00021165819,0.00013139502,0.00017882102,0.000877154],"category_scores_gemma":[0.00007654426,0.00012672023,0.000088011635,0.00022438962,0.00014539891,0.00012533416,0.00013332133,0.00012098282,0.00020236336],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003513866,0.00015237089,0.13284144,0.00012882486,0.000051736137,0.0017029931,0.0003426072,0.00031115694,0.8338448,0.00063850917,0.00082406827,0.02881008],"study_design_scores_gemma":[0.000016814336,0.00017431707,0.9818381,0.0000071003597,0.000013052301,0.0010304347,0.0001062946,0.00031676318,0.0132861165,0.00013494324,0.003070373,0.0000056625854],"about_ca_topic_score_codex":0.0012445232,"about_ca_topic_score_gemma":0.0022744222,"teacher_disagreement_score":0.0012445232,"about_ca_system_score_codex":0.0001874434,"about_ca_system_score_gemma":0.00007086631,"threshold_uncertainty_score":0.0029343367},"labels":[],"label_agreement":null},{"id":"W2017874065","doi":"10.1086/428653","title":"Raman and Infrared Emission Spectra of Hydrogenated Amorphous Carbon: Insight into the Origin of the 6-14 Micron Infrared Emission Bands","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Diamond and Carbon-based Materials Research","field":"Materials Science","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Infrared; Raman spectroscopy; Emission spectrum; Infrared spectroscopy; Amorphous carbon; Amorphous solid; Spectral line; Analytical Chemistry (journal); Polycyclic aromatic hydrocarbon; Physics; Photochemistry; Chemistry; Optics; Astronomy; Crystallography; Organic chemistry; Astrobiology","score_opus":0.00786339333307535,"score_gpt":0.23882722589397432,"score_spread":0.23096383256089897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017874065","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967699,0.00023590669,0.0019238137,0.000017938271,0.0000030721733,0.0000035057997,0.00006214499,0.000023548757,0.00096021773],"genre_scores_gemma":[0.9950944,0.00012412772,0.0038117697,0.000008013376,0.0000032621128,0.0000033492984,0.000097180746,0.000006911612,0.00085108104],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999311,0.0000072955954,0.000002896764,0.000012896079,0.000030217176,0.000015651502],"domain_scores_gemma":[0.99983585,0.00005800185,0.000021025317,0.000013236647,0.000053319734,0.000018644496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015665563,0.00016399146,0.000075714124,0.00031575194,0.00013626365,0.00016101387,0.00022050939,0.00016636049,0.00085311197],"category_scores_gemma":[0.00016346018,0.00007683906,0.00010402945,0.00014036402,0.0002038794,0.00015564183,0.000112867965,0.00023406083,0.00012709586],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002083846,0.000015166043,0.0015485778,0.000014403166,0.0000043665254,0.000056773362,0.00004291429,0.000096313524,0.99600756,0.00009878408,0.000011659346,0.0020825625],"study_design_scores_gemma":[0.0000044442177,0.00017147408,0.03250562,0.0000060682837,0.000013405078,0.00021395335,0.00012761929,0.0016356984,0.96437544,0.00011061806,0.00082589046,0.000009734356],"about_ca_topic_score_codex":0.0008696748,"about_ca_topic_score_gemma":0.0012761294,"teacher_disagreement_score":0.0008696748,"about_ca_system_score_codex":0.00011324583,"about_ca_system_score_gemma":0.00007035866,"threshold_uncertainty_score":0.0028539896},"labels":[],"label_agreement":null},{"id":"W2017875708","doi":"10.1088/0004-637x/748/2/129","title":"GALAXY SCALE LENSES IN THE RCS2. I. FIRST CATALOG OF CANDIDATE STRONG LENSES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; University of Toronto","funders":"","keywords":"Galaxy; Lens (geology); Redshift; Dark matter; Gravitational lens; Range (aeronautics); Simple lens","score_opus":0.010036337236908374,"score_gpt":0.2203089357047481,"score_spread":0.21027259846783974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017875708","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8415097,0.0060221907,0.0015493302,0.0005915823,0.00006796306,0.00013305049,0.06529889,0.00076755066,0.08405984],"genre_scores_gemma":[0.89808905,0.0011540232,0.0031145157,0.00019342541,0.00008922955,0.00006612544,0.083038956,0.00010858423,0.014146112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99944025,0.000031610398,0.00003418267,0.00011495106,0.00021577634,0.00016324366],"domain_scores_gemma":[0.9981012,0.00015786928,0.00037617213,0.00029356667,0.00053336326,0.0005377444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046156585,0.00045253037,0.00027233656,0.009117582,0.00083920796,0.001491197,0.0004218398,0.00028412463,0.010451243],"category_scores_gemma":[0.001207141,0.00018520546,0.0003195041,0.00636137,0.0002893106,0.00052887044,0.0012240397,0.00024879284,0.0034320415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005355879,0.0001232047,0.77823055,0.0003203758,0.00014025417,0.00077022554,0.0007108899,0.0005410719,0.016761374,0.0053799828,0.061089177,0.13539733],"study_design_scores_gemma":[0.000013888064,0.000031729487,0.9268204,0.000039364848,0.00003463578,0.0008081796,0.00034761062,0.00027842008,0.0015804468,0.00035116271,0.069678545,0.000015598056],"about_ca_topic_score_codex":0.025724687,"about_ca_topic_score_gemma":0.060843118,"teacher_disagreement_score":0.025724687,"about_ca_system_score_codex":0.0008517121,"about_ca_system_score_gemma":0.0013486659,"threshold_uncertainty_score":0.051149905},"labels":[],"label_agreement":null},{"id":"W2017995773","doi":"10.1088/0004-637x/745/2/109","title":"THE TIMING OF NINE GLOBULAR CLUSTER PULSARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":202,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Globular cluster; Pulsar; Astrophysics; Astronomy; Cluster (spacecraft); Horizontal branch; Star cluster; Stars","score_opus":0.015400487107644273,"score_gpt":0.3210826221610829,"score_spread":0.30568213505343866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2017995773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99778086,0.00008346315,0.0006598608,0.000028300447,0.000020965103,0.000010532972,0.0004756331,0.00006230628,0.00087815087],"genre_scores_gemma":[0.9938146,0.00008390077,0.0029981262,0.000022849577,0.000026222142,0.000016200289,0.0023546726,0.000023502505,0.00066004175],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965405,0.000028480677,0.00002949706,0.000120914294,0.00011177605,0.0000551595],"domain_scores_gemma":[0.99928975,0.0001267838,0.00013898658,0.00011053829,0.00016798446,0.00016588606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037507675,0.0001789191,0.00025498917,0.001287468,0.0007618995,0.00047332092,0.00037099264,0.0004241111,0.0010696286],"category_scores_gemma":[0.0011868044,0.00016893506,0.00013131848,0.001188759,0.0003005582,0.00025000196,0.00059538236,0.0002998129,0.00028058898],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031136087,0.00008235597,0.91215944,0.00006112476,0.00006460071,0.0005798726,0.0011050373,0.0015214772,0.039005596,0.00039717427,0.0010071367,0.04370483],"study_design_scores_gemma":[0.000022888285,0.00012439252,0.9899748,0.000006632416,0.00002807722,0.00023674515,0.00010495999,0.001477559,0.0045873504,0.000099070465,0.0033190036,0.000018500585],"about_ca_topic_score_codex":0.006168124,"about_ca_topic_score_gemma":0.0106533645,"teacher_disagreement_score":0.006168124,"about_ca_system_score_codex":0.00075194245,"about_ca_system_score_gemma":0.00027086263,"threshold_uncertainty_score":0.0122644305},"labels":[],"label_agreement":null},{"id":"W2018000395","doi":"10.1086/343115","title":"X‐Ray versus Optical Observations of Active Galactic Nuclei: Evidence for Large Grains?","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Active galactic nucleus; Galaxy; Torus; Extinction (optical mineralogy); Line-of-sight; Luminous infrared galaxy; Peculiar galaxy; Accretion (finance); Line (geometry)","score_opus":0.05505588993197578,"score_gpt":0.2739677919971985,"score_spread":0.21891190206522274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018000395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99544805,0.0011401221,0.000453864,0.00014342487,0.000016553295,0.000006580421,0.00011021294,0.000020684041,0.00266068],"genre_scores_gemma":[0.99909604,0.00020962558,0.00019852383,0.000093773786,0.00004297566,0.0000055449477,0.00010466101,0.0000047365443,0.0002440053],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966836,0.00002997572,0.000025078538,0.00012734633,0.00007387277,0.000075408985],"domain_scores_gemma":[0.99806327,0.00059128314,0.000739739,0.0002362351,0.00014142354,0.00022804206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003840337,0.0002273839,0.00033541102,0.0007757509,0.00031323396,0.0009969325,0.0004546909,0.0005468261,0.002208557],"category_scores_gemma":[0.001668675,0.0002225239,0.00022099519,0.00053301995,0.0006760915,0.0008452683,0.0005520423,0.0002305564,0.00040484197],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005213617,0.0000884294,0.939537,0.00008703593,0.000110574605,0.00039286984,0.00031202968,0.000060106962,0.047196418,0.00045233188,0.00022947518,0.011012356],"study_design_scores_gemma":[0.0000116857345,0.000050697967,0.9959806,0.00000906053,0.000030559844,0.00043043736,0.00017020709,0.00010477178,0.0021753842,0.00023319595,0.0008001085,0.0000031943275],"about_ca_topic_score_codex":0.0016152997,"about_ca_topic_score_gemma":0.00313133,"teacher_disagreement_score":0.002208557,"about_ca_system_score_codex":0.00026289068,"about_ca_system_score_gemma":0.00007030608,"threshold_uncertainty_score":0.0073883533},"labels":[],"label_agreement":null},{"id":"W2018048585","doi":"10.1088/0004-637x/765/1/59","title":"AN ANALYSIS OF THE DEUTERIUM FRACTIONATION OF STAR-FORMING CORES IN THE PERSEUS MOLECULAR CLOUD","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"","keywords":"Deuterium; Ophiuchus; Fractionation; Molecular cloud; Star formation; Protostar; Astrochemistry","score_opus":0.007596817672084595,"score_gpt":0.24566414881652143,"score_spread":0.23806733114443684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018048585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997352,0.000041478685,0.00005044695,0.0000034594277,3.695106e-7,7.6959907e-7,0.000064665306,0.0000025014608,0.000101035104],"genre_scores_gemma":[0.99953437,0.000033644974,0.00014657005,0.00000439142,0.0000015464309,9.1781993e-7,0.00021684382,0.0000019517458,0.00005981945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999546,0.0000054303227,0.0000023438508,0.000017063665,0.000009753788,0.000010763529],"domain_scores_gemma":[0.99981815,0.000028113083,0.00006401917,0.000019010531,0.00002912229,0.000041670824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013620287,0.00020727153,0.00014297805,0.000940063,0.00018639489,0.00022625396,0.00021201791,0.00009720119,0.00028876358],"category_scores_gemma":[0.0003365977,0.00011826626,0.00011680211,0.000517884,0.0001589804,0.00013068915,0.00023375817,0.00006703993,0.000064721375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000117541604,0.000012219472,0.96324855,0.0000135322125,0.000055953973,0.00018118856,0.00016916549,0.0010494099,0.030672116,0.00010635925,0.000058838184,0.004315146],"study_design_scores_gemma":[0.0000046848236,0.000023700413,0.9956624,0.0000021986389,0.000010667099,0.00008097564,0.0000625031,0.0014112096,0.0024606583,0.000038976712,0.00023947645,0.0000024255337],"about_ca_topic_score_codex":0.013425918,"about_ca_topic_score_gemma":0.018086176,"teacher_disagreement_score":0.013425918,"about_ca_system_score_codex":0.0003635821,"about_ca_system_score_gemma":0.00014312183,"threshold_uncertainty_score":0.02669555},"labels":[],"label_agreement":null},{"id":"W2018140110","doi":"10.1086/430048","title":"Discovering Gravitational Lenses through Measurements of Their Time Delays","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Quasar; Gravitational lens; Lens (geology); Window function; Computer science; Gravitational field; Physics; Field of view; Function (biology); Window (computing); Gravitation; Time domain; Field (mathematics); Optics; Astronomy; Mathematics; Computer vision","score_opus":0.017468375067510426,"score_gpt":0.22921024002172055,"score_spread":0.21174186495421013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018140110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91354185,0.0011169259,0.07871369,0.00022139073,0.000020322997,0.000028631173,0.00095143256,0.0002289665,0.0051767286],"genre_scores_gemma":[0.9793397,0.00032703514,0.019491054,0.000011847675,0.000012259321,0.0000056722074,0.0002850988,0.000008723589,0.0005186156],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998878,0.000021471158,0.0000048077336,0.000031253163,0.0000279441,0.00002677159],"domain_scores_gemma":[0.9983171,0.0008598593,0.0005243863,0.000119764445,0.000103257975,0.00007566065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059490505,0.00021739802,0.0001753101,0.001072363,0.00021169352,0.0006092065,0.0003214307,0.00020437203,0.0020523767],"category_scores_gemma":[0.003421065,0.0001262909,0.00018851664,0.0012970973,0.00021560832,0.000798591,0.00038264922,0.0002060027,0.0002889517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005594047,0.0000908966,0.66107327,0.00030714547,0.00029620095,0.00031330288,0.00025683927,0.064511605,0.075792916,0.028807947,0.0012258218,0.16676466],"study_design_scores_gemma":[0.00008319927,0.0005585938,0.62833273,0.000051749448,0.00023340312,0.0015113017,0.00055918086,0.24327573,0.058945302,0.04874009,0.017569514,0.00013932062],"about_ca_topic_score_codex":0.0036531445,"about_ca_topic_score_gemma":0.0077451477,"teacher_disagreement_score":0.0036531445,"about_ca_system_score_codex":0.00038244773,"about_ca_system_score_gemma":0.00024795643,"threshold_uncertainty_score":0.0072637796},"labels":[],"label_agreement":null},{"id":"W2018179836","doi":"10.1088/0004-637x/800/2/122","title":"REVISED MASS-TO-LIGHT RATIOS FOR NEARBY GALAXY GROUPS AND CLUSTERS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Astrophysics; Physics; Photometry (optics); Stellar mass; Galaxy; Sky; Galaxy cluster; Brightest cluster galaxy; Astronomy; Redshift; Cluster (spacecraft); Star formation; Stars","score_opus":0.011833146925680651,"score_gpt":0.22525539353799628,"score_spread":0.21342224661231562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018179836","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98780036,0.0005373745,0.0038906534,0.000042306572,0.000013625513,0.000024441888,0.0034433452,0.00042324874,0.003824613],"genre_scores_gemma":[0.9915774,0.00010136523,0.0036278984,0.000015522375,0.00001605603,0.000017075035,0.0037676357,0.00011825394,0.0007587841],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994947,0.00006294385,0.000052865213,0.00016590473,0.00015333161,0.00007026115],"domain_scores_gemma":[0.9981046,0.0003695853,0.00048388253,0.00047830853,0.00040243944,0.00016118967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00093551824,0.00045538906,0.00033269436,0.0048913807,0.00037047436,0.0008904002,0.00058459974,0.00032017098,0.0030636496],"category_scores_gemma":[0.004106186,0.0002040844,0.00054742605,0.0016773824,0.00022368279,0.00050067983,0.00070947193,0.00025719102,0.002007713],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022225842,0.000030209116,0.93141204,0.00009639391,0.00016219824,0.00014741678,0.0006326682,0.0039890506,0.01338177,0.001157935,0.0016328667,0.04713526],"study_design_scores_gemma":[0.000009414031,0.000076721044,0.9857438,0.00001272031,0.00006178859,0.00028268452,0.00018349619,0.005875127,0.0030985912,0.0005155783,0.004122336,0.000017590644],"about_ca_topic_score_codex":0.004051599,"about_ca_topic_score_gemma":0.0042527025,"teacher_disagreement_score":0.0048913807,"about_ca_system_score_codex":0.0004150607,"about_ca_system_score_gemma":0.00018472731,"threshold_uncertainty_score":0.010248899},"labels":[],"label_agreement":null},{"id":"W2018312917","doi":"10.1086/382778","title":"Further Multiwavelength Observations of the SSA 22 Lyα‐Emitting Blob","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Astronomy; Millimeter; Galaxy; Telescope; Active galactic nucleus; Space Telescope Imaging Spectrograph; James Clerk Maxwell Telescope; Observatory; Spectrograph; Quasar; Star formation; Hubble space telescope; Spectral line","score_opus":0.012155564691435247,"score_gpt":0.2120341321319343,"score_spread":0.19987856744049906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018312917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9881196,0.00043089734,0.0011722688,0.00007647138,0.000016507243,0.000024910769,0.0012426914,0.00016113762,0.008755389],"genre_scores_gemma":[0.9886989,0.000260919,0.0033892202,0.000096554686,0.000039972037,0.000030260082,0.0027871947,0.000036300287,0.004660654],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994695,0.0000025023915,0.0000015927542,0.000011084262,0.000014167742,0.000023719895],"domain_scores_gemma":[0.99973375,0.000016346807,0.00007743532,0.000031199663,0.000033041993,0.000108268025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011350691,0.00030330577,0.00023613086,0.00086449954,0.00040574372,0.00048358206,0.00020569711,0.00020586485,0.0047995746],"category_scores_gemma":[0.000121581295,0.00015372061,0.00030685656,0.00062816316,0.00010318218,0.00028950762,0.00035839036,0.00039431918,0.0009389553],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041927132,0.00034909367,0.41781867,0.00018316643,0.00023721858,0.0015558711,0.0018093487,0.00090836023,0.5065751,0.0007100637,0.00440843,0.06502543],"study_design_scores_gemma":[0.000010513062,0.00011784659,0.9891328,0.000009036348,0.000027246375,0.0004674021,0.00010346623,0.000321055,0.0025858704,0.00008634003,0.0071299714,0.000008507536],"about_ca_topic_score_codex":0.004525563,"about_ca_topic_score_gemma":0.017640967,"teacher_disagreement_score":0.0047995746,"about_ca_system_score_codex":0.00024690566,"about_ca_system_score_gemma":0.00010683223,"threshold_uncertainty_score":0.01605618},"labels":[],"label_agreement":null},{"id":"W2018395159","doi":"10.1088/0004-637x/729/1/49","title":"ASTROMETRIC MICROLENSING BY LOCAL DARK MATTER SUBHALOS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute","funders":"","keywords":"Gravitational microlensing; Dark matter; Halo; Baryonic dark matter; Solar mass; Gravitational lens","score_opus":0.013572286897408638,"score_gpt":0.2350786255273796,"score_spread":0.22150633862997096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018395159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97810566,0.0001442372,0.016632963,0.000042893123,0.0000034540303,0.000010906473,0.00015881035,0.00020184414,0.004699099],"genre_scores_gemma":[0.9979746,0.000060688002,0.0015431155,0.000008215789,0.0000028013958,0.000004151201,0.000072673596,0.000015889902,0.0003178093],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999125,0.00001717989,0.0000033356737,0.000018491808,0.000024840248,0.000023733695],"domain_scores_gemma":[0.9993936,0.0002294309,0.00019852257,0.00006489708,0.00003433083,0.00007923727],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029333646,0.0003011789,0.00018047572,0.00054731494,0.00024386913,0.00059417944,0.00040254777,0.00022973526,0.000920925],"category_scores_gemma":[0.001591447,0.00019662571,0.00046688342,0.00031005192,0.00034024732,0.0005251857,0.0006437859,0.00022129124,0.00013213519],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011143659,0.000053052274,0.39155942,0.00006142152,0.00019391564,0.00072035415,0.0002496597,0.5428812,0.01793444,0.028289132,0.00067779707,0.017268112],"study_design_scores_gemma":[0.0000149271345,0.0000344348,0.09008744,0.00001337274,0.000030044936,0.00018789066,0.000050124992,0.89578295,0.006437196,0.0062876553,0.0010528847,0.000021108472],"about_ca_topic_score_codex":0.0045105717,"about_ca_topic_score_gemma":0.0032251887,"teacher_disagreement_score":0.0045105717,"about_ca_system_score_codex":0.00070666516,"about_ca_system_score_gemma":0.00016665978,"threshold_uncertainty_score":0.008968651},"labels":[],"label_agreement":null},{"id":"W2018460911","doi":"10.1088/0004-637x/777/1/7","title":"DISCOVERY OF A LARGE POPULATION OF ULTRALUMINOUS X-RAY SOURCES IN THE BULGELESS GALAXIES NGC 337 AND ESO 501-23","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Luminosity; Population; Star formation; Bulge; Active galactic nucleus; Flux (metallurgy); Astronomy; Luminosity function","score_opus":0.007984124159136137,"score_gpt":0.22049866417356825,"score_spread":0.21251454001443212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018460911","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99957925,0.000048087324,0.00007555147,0.000016444721,7.1670473e-7,0.0000020615512,0.00003516443,0.0000055733112,0.00023708654],"genre_scores_gemma":[0.9990662,0.00006677325,0.0003515059,0.000022879198,0.0000051147513,0.0000069433163,0.00025652617,0.0000029967648,0.00022112338],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987113,0.000013350326,0.000008015144,0.000034288714,0.00003831985,0.00003490513],"domain_scores_gemma":[0.99950004,0.00007595894,0.00019397015,0.00005338062,0.00004237823,0.0001341858],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026275514,0.00022698406,0.00024142147,0.0008413847,0.0004597871,0.0007038984,0.00040550964,0.00026227033,0.0009092686],"category_scores_gemma":[0.00043164162,0.00017789824,0.00016965793,0.000489585,0.0005183306,0.00030015758,0.0007354821,0.00025033063,0.00017676571],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018753459,0.00004550555,0.9622903,0.000016962022,0.000040260165,0.0006874004,0.00064687006,0.00015204724,0.028267963,0.00041324852,0.0001534922,0.007098433],"study_design_scores_gemma":[0.000007245783,0.00005563894,0.99708873,0.0000059799013,0.000019871602,0.0005199597,0.00019229174,0.0001573849,0.0014016839,0.000056873974,0.0004884083,0.00000586046],"about_ca_topic_score_codex":0.0042216135,"about_ca_topic_score_gemma":0.008044131,"teacher_disagreement_score":0.0042216135,"about_ca_system_score_codex":0.0003558989,"about_ca_system_score_gemma":0.0001718566,"threshold_uncertainty_score":0.0083940625},"labels":[],"label_agreement":null},{"id":"W2018609579","doi":"10.1088/0004-637x/765/1/18","title":"RESOLVED DEPLETION ZONES AND SPATIAL DIFFERENTIATION OF N<sub>2</sub>H<sup>+</sup>AND N<sub>2</sub>D<sup>+</sup>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; RADIUS; Plateau de Bure Interferometer; Protostar; Submillimeter Array; Envelope (radar); Astrophysics; Atomic physics; Star formation; Stars","score_opus":0.007344530072783763,"score_gpt":0.20261331412093758,"score_spread":0.19526878404815382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018609579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97436476,0.0007511043,0.006487654,0.0001244686,0.00002796552,0.000020963991,0.000993072,0.00013397743,0.017096024],"genre_scores_gemma":[0.993885,0.0001305763,0.0017792034,0.00005046485,0.000007951574,0.00001671799,0.00053905975,0.00003250893,0.0035584406],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999516,0.0000021133285,0.0000017090525,0.000020212703,0.000011193025,0.000013211089],"domain_scores_gemma":[0.9998211,0.00004380074,0.00004880821,0.00001570534,0.000039899023,0.000030640665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012304338,0.00013245434,0.00008612646,0.000595093,0.00028626804,0.00061216246,0.00049019203,0.00028117653,0.0043966193],"category_scores_gemma":[0.00042276856,0.00019625713,0.00010139025,0.0003238234,0.00040607477,0.0005507192,0.0004173486,0.00029003722,0.00044583337],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019991642,0.000108253385,0.04581076,0.00016464725,0.00004314696,0.00040121694,0.0007336686,0.0051662344,0.912669,0.014069327,0.0013604205,0.017474107],"study_design_scores_gemma":[0.00011238967,0.00014852794,0.4967208,0.000046665882,0.0000670579,0.0010304368,0.0012639812,0.04553963,0.42840388,0.011563672,0.015025738,0.000077291006],"about_ca_topic_score_codex":0.0026340617,"about_ca_topic_score_gemma":0.0035879114,"teacher_disagreement_score":0.0043966193,"about_ca_system_score_codex":0.0005007371,"about_ca_system_score_gemma":0.00018759572,"threshold_uncertainty_score":0.014708161},"labels":[],"label_agreement":null},{"id":"W2018625833","doi":"10.1088/0004-637x/800/1/32","title":"HERCULES X-1: USING ECLIPSE TO MEASURE THE X-RAY CORONA","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Neutron star; Corona (planetary geology); Hydrostatic equilibrium; Accretion (finance); X-ray binary; Flux (metallurgy); Outflow; Eclipse; Compton scattering; Scattering; Astronomy; Optics","score_opus":0.0604696681957145,"score_gpt":0.27218666999350216,"score_spread":0.21171700179778766,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018625833","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99467385,0.00028656918,0.00032799182,0.000014140109,0.000004979457,0.000017862758,0.0013682621,0.00011247109,0.0031939114],"genre_scores_gemma":[0.99480975,0.00014542426,0.0013345225,0.000021111244,0.00001104995,0.0000104104765,0.0028364132,0.00004908427,0.00078227575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989283,0.00001182772,0.000004243774,0.000044007465,0.00002429637,0.00002276407],"domain_scores_gemma":[0.99977535,0.000028539793,0.00007372611,0.000038759223,0.000038569033,0.000045007477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002497699,0.0003120402,0.00023238242,0.00092584704,0.00022334182,0.00033933026,0.0002588202,0.00028089358,0.0013512683],"category_scores_gemma":[0.0003046101,0.00015485489,0.00016802098,0.00046929874,0.000100118115,0.0002499581,0.00033486803,0.00018251534,0.00033726275],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013304034,0.0002059075,0.765001,0.00022917752,0.00024121377,0.0011258794,0.0003567102,0.0028920171,0.19682316,0.00053307024,0.0029300586,0.028331239],"study_design_scores_gemma":[0.000018226408,0.000092995244,0.99288213,0.000008900403,0.000021499749,0.0003152154,0.000036022408,0.0016698224,0.0035303563,0.00003226907,0.0013857071,0.000006898351],"about_ca_topic_score_codex":0.0052129794,"about_ca_topic_score_gemma":0.010695983,"teacher_disagreement_score":0.0052129794,"about_ca_system_score_codex":0.00026658588,"about_ca_system_score_gemma":0.000097035794,"threshold_uncertainty_score":0.010365307},"labels":[],"label_agreement":null},{"id":"W2018716293","doi":"10.1086/374598","title":"Planet Migration and Binary Companions: The Case of HD 80606b","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":676,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planet; Orbital eccentricity; Orbit (dynamics); Eccentricity (behavior); Exoplanet; Giant planet; Dissipation; Tidal acceleration; Tidal heating; Planetary system","score_opus":0.012419456286776697,"score_gpt":0.22667990889166986,"score_spread":0.21426045260489315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018716293","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941782,0.00033144356,0.00008438509,0.0004391081,0.000007438309,0.0000053563253,0.00006437501,0.000007675472,0.0048819906],"genre_scores_gemma":[0.999027,0.00013638237,0.000106533036,0.000025377085,0.000012397776,0.0000023830369,0.00009084911,0.0000051464763,0.0005939978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998217,0.00004091334,0.000009932975,0.000027351174,0.000024529874,0.000075559066],"domain_scores_gemma":[0.99922836,0.00030543594,0.00019535616,0.000056787027,0.00004300845,0.00017111913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055488304,0.00029481488,0.0005976816,0.0011270688,0.0025084633,0.0013971645,0.0005124508,0.0014977946,0.0035251833],"category_scores_gemma":[0.001943004,0.00020070809,0.0004363943,0.0012603465,0.0009744161,0.0009988814,0.0015732253,0.0006138336,0.00039738129],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001739076,0.00077983685,0.858941,0.00023484141,0.00017040539,0.049562976,0.004637193,0.015442649,0.009470041,0.03386785,0.0068925847,0.018261403],"study_design_scores_gemma":[0.00048100768,0.0004976346,0.86334455,0.00011542516,0.00026933613,0.015564138,0.009631073,0.07652527,0.0024269954,0.01801101,0.013009243,0.00012437649],"about_ca_topic_score_codex":0.0475709,"about_ca_topic_score_gemma":0.035432585,"teacher_disagreement_score":0.0475709,"about_ca_system_score_codex":0.0010626703,"about_ca_system_score_gemma":0.00045327665,"threshold_uncertainty_score":0.09458798},"labels":[],"label_agreement":null},{"id":"W2018907465","doi":"10.1088/0004-637x/736/1/74","title":"THE LIGHT CURVE OF HERCULES X-1 AS OBSERVED BY THE<i>ROSSI X-RAY TIMING EXPLORER</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Light curve; Astrophysics; Phase (matter); X-ray; Orbital period; Range (aeronautics); Astronomy; Stars; Optics","score_opus":0.04016898233276088,"score_gpt":0.2316253669044323,"score_spread":0.1914563845716714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018907465","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98801315,0.00030190783,0.00021200562,0.00012696226,0.000012378549,0.000016675327,0.0057864175,0.0003479265,0.0051825526],"genre_scores_gemma":[0.9835844,0.00022420916,0.00062828144,0.0000638051,0.000042521402,0.00001755144,0.013249155,0.00011620586,0.0020738016],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988484,0.000010757721,0.0000047347535,0.00003269639,0.000033425313,0.000033590975],"domain_scores_gemma":[0.9992293,0.000090875306,0.00025198574,0.00007595589,0.00018982119,0.00016208141],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000252912,0.00040696008,0.00023404296,0.0022696522,0.00028958847,0.0005061441,0.00027700412,0.00031501736,0.0026474409],"category_scores_gemma":[0.00049127446,0.00012204314,0.00019543138,0.001295755,0.00018300327,0.00026182013,0.00039215054,0.0003508113,0.0009939029],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009350234,0.00024660074,0.84989053,0.00025231997,0.00024225489,0.00095820794,0.00080201734,0.0048478157,0.06222933,0.0010344654,0.02710881,0.05145269],"study_design_scores_gemma":[0.000006803064,0.000035482946,0.9937186,0.000009278852,0.000011167024,0.00014050704,0.000044243418,0.0012845129,0.0009822977,0.000056540346,0.0037007434,0.000009914857],"about_ca_topic_score_codex":0.010409001,"about_ca_topic_score_gemma":0.011983998,"teacher_disagreement_score":0.010409001,"about_ca_system_score_codex":0.00058100966,"about_ca_system_score_gemma":0.0001520845,"threshold_uncertainty_score":0.020696819},"labels":[],"label_agreement":null},{"id":"W2018926820","doi":"10.1086/381260","title":"PSR J1909-3744: A Binary Millisecond Pulsar with a Very Small Duty Cycle","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration; Commonwealth Scientific and Industrial Research Organisation; National Science Foundation","keywords":"Millisecond pulsar; Physics; Pulsar; Astrophysics; Astronomy; Gravitational wave; Binary pulsar; Proper motion; Duty cycle; Mass ratio; Stars","score_opus":0.01031254835576144,"score_gpt":0.26895914112932384,"score_spread":0.2586465927735624,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018926820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973176,0.0003693087,0.00046519836,0.00007348184,0.00003240886,0.000009606216,0.00014960188,0.000055801152,0.0015269174],"genre_scores_gemma":[0.99762744,0.00014884476,0.0010432007,0.00003441873,0.000040288724,0.0000043355494,0.0004106844,0.000008160428,0.0006826946],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.000009461213,0.000008246143,0.000025107725,0.000046090903,0.000033195975],"domain_scores_gemma":[0.9998503,0.000010057627,0.00006196268,0.000021152891,0.000018138708,0.00003837694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016235311,0.00021233756,0.00028940442,0.00041434474,0.00048897584,0.00037455544,0.0003824718,0.0002880108,0.00081291335],"category_scores_gemma":[0.00032780643,0.00008741377,0.000081553924,0.00036274307,0.0003097653,0.00030573842,0.00042002808,0.000261615,0.00042098598],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001443721,0.00031961603,0.21467839,0.00023660962,0.00014303399,0.010802396,0.00069715944,0.0011077106,0.66008234,0.0047800858,0.0052154646,0.100493506],"study_design_scores_gemma":[0.00023715563,0.0033272211,0.5734632,0.000034946013,0.00022242597,0.043930076,0.0004435694,0.008283369,0.29115587,0.0032730645,0.07552427,0.000104746745],"about_ca_topic_score_codex":0.0015802995,"about_ca_topic_score_gemma":0.0017011637,"teacher_disagreement_score":0.0015802995,"about_ca_system_score_codex":0.00030255024,"about_ca_system_score_gemma":0.00016039847,"threshold_uncertainty_score":0.003142178},"labels":[],"label_agreement":null},{"id":"W2018947165","doi":"10.1086/590660","title":"A Glimpse into the Past: The Recent Evolution of Globular Clusters","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Globular cluster; Elliptical galaxy; Galaxy; Luminosity function; Luminosity; Redshift; Stellar population","score_opus":0.007264073012017555,"score_gpt":0.20392997910854332,"score_spread":0.19666590609652576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018947165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91147053,0.060012225,0.0010818256,0.013174817,0.00027461856,0.000010056448,0.0017151552,0.00008463151,0.012176151],"genre_scores_gemma":[0.9668287,0.02543061,0.0014690831,0.0019457383,0.0005833097,0.000006183157,0.0012188015,0.00007749077,0.0024400766],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985635,0.000021984211,0.000015330277,0.00004948561,0.000026489686,0.000030264377],"domain_scores_gemma":[0.99832517,0.00035157867,0.00042659734,0.00017425316,0.00032685275,0.00039552996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007514718,0.00019670636,0.00029017578,0.0017124187,0.00096694584,0.0021353308,0.00043867488,0.0007626437,0.0017597852],"category_scores_gemma":[0.0021691683,0.00018660276,0.00017548552,0.0022986585,0.0013601338,0.0028154897,0.0009971467,0.0012865155,0.00038436314],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052064745,0.000120160796,0.7589304,0.0007803261,0.00027594448,0.0019580247,0.01402344,0.0009353336,0.0100267595,0.016618254,0.012139867,0.18367082],"study_design_scores_gemma":[0.0000042861443,0.0000716886,0.9223225,0.00023814049,0.000046447745,0.0013365856,0.0028495137,0.00022398384,0.0006200284,0.0034653072,0.06878348,0.000037914968],"about_ca_topic_score_codex":0.013789029,"about_ca_topic_score_gemma":0.024022078,"teacher_disagreement_score":0.013789029,"about_ca_system_score_codex":0.001023748,"about_ca_system_score_gemma":0.00028235826,"threshold_uncertainty_score":0.02741754},"labels":[],"label_agreement":null},{"id":"W2018972779","doi":"10.1088/0004-637x/732/2/86","title":"SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC). III. CHAMAELEON-I","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Photometry (optics); Spectrograph; Spitzer Space Telescope; Stars; Stellar classification; Brown dwarf; Cluster (spacecraft); Telescope","score_opus":0.014143596551980553,"score_gpt":0.218818301528881,"score_spread":0.20467470497690043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2018972779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963961,0.0005670624,0.00031427306,0.00001684217,0.0000118368225,0.000019672041,0.00043812164,0.00002479379,0.002211278],"genre_scores_gemma":[0.99566865,0.00021618673,0.0010086601,0.000016458083,0.000013858988,0.000013378259,0.0019362636,0.0000056160093,0.0011209637],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998523,0.000010102029,0.000009200863,0.000048724673,0.000034538614,0.00004509597],"domain_scores_gemma":[0.999461,0.000042673397,0.00017093582,0.000054781078,0.00008042681,0.00019020484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028588023,0.00018778615,0.00021612574,0.0012347638,0.00084330904,0.00055722886,0.00026020827,0.00016416026,0.0016593342],"category_scores_gemma":[0.00038862033,0.00008318617,0.00016316447,0.0010668768,0.00024720177,0.00033474388,0.0007772485,0.0001462238,0.00022105717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022151787,0.000030257543,0.9596553,0.00006928332,0.000030670897,0.00044026037,0.0006135669,0.00028761537,0.013689204,0.00064333365,0.0007217157,0.023597203],"study_design_scores_gemma":[0.0000049255937,0.00006923004,0.9945862,0.000008087589,0.000010996781,0.00038427862,0.00027875026,0.0002584328,0.0009965823,0.00008684437,0.003310401,0.0000051846973],"about_ca_topic_score_codex":0.013280641,"about_ca_topic_score_gemma":0.033147227,"teacher_disagreement_score":0.013280641,"about_ca_system_score_codex":0.00051443215,"about_ca_system_score_gemma":0.00028918264,"threshold_uncertainty_score":0.026406646},"labels":[],"label_agreement":null},{"id":"W2019016642","doi":"10.1088/0004-637x/782/1/33","title":"THE PAN-STARRS1 MEDIUM-DEEP SURVEY: THE ROLE OF GALAXY GROUP ENVIRONMENT IN THE STAR FORMATION RATE VERSUS STELLAR MASS RELATION AND QUIESCENT FRACTION OUT TO<i>z</i>∼ 0.8","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; National Central University; Space Telescope Science Institute; National Science Council; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; Stellar mass; Star formation; Galaxy; Quenching (fluorescence); Astronomy","score_opus":0.007621965638541085,"score_gpt":0.19844187911879313,"score_spread":0.19081991348025204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019016642","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980909,0.0001421452,0.00017703554,0.00002551906,0.0000010710575,0.0000028634952,0.000989874,0.00002612328,0.0005444775],"genre_scores_gemma":[0.99721813,0.000053620905,0.00019987172,0.000012689017,0.000005679877,0.0000034360587,0.0022879976,0.000009977634,0.0002085415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998641,0.000023441362,0.0000065682543,0.000056097873,0.000017503824,0.00003224749],"domain_scores_gemma":[0.99900085,0.00020027255,0.0003685006,0.00012107937,0.00007020112,0.00023923539],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046022912,0.00026419325,0.0002805157,0.0010272518,0.00016458688,0.0004880776,0.00030599325,0.00021571298,0.001152633],"category_scores_gemma":[0.00086505484,0.00015134887,0.00027189736,0.00064905797,0.00021932386,0.0003373403,0.0006681163,0.00020824574,0.00030994375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011182014,0.000019393514,0.9904073,0.000026963564,0.00005910884,0.00004966704,0.00012372075,0.00036636033,0.004317222,0.00013131202,0.00025076314,0.0041363775],"study_design_scores_gemma":[0.0000025092934,0.000012587647,0.9992397,0.0000013232192,0.000007751861,0.000025198773,0.000025131169,0.0003071034,0.00015244985,0.000019004025,0.00020583309,0.0000013883482],"about_ca_topic_score_codex":0.005989992,"about_ca_topic_score_gemma":0.00842339,"teacher_disagreement_score":0.005989992,"about_ca_system_score_codex":0.00020347624,"about_ca_system_score_gemma":0.000106943124,"threshold_uncertainty_score":0.01191026},"labels":[],"label_agreement":null},{"id":"W2019124046","doi":"10.1086/375832","title":"The Infrared Counterpart to the Anomalous X-Ray Pulsar 1RXS J170849-400910","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Pulsar; Physics; Astrophysics; Infrared; Telescope; Flux (metallurgy); Astronomy; Neutron star; Black-body radiation; Optics; Radiation","score_opus":0.009195711425947165,"score_gpt":0.22763048282944456,"score_spread":0.2184347714034974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019124046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99838674,0.00017669091,0.00019651758,0.00002934431,0.0000074038107,0.0000025740046,0.00007697633,0.000013108927,0.0011106528],"genre_scores_gemma":[0.99783653,0.00018824602,0.0007565995,0.000032154432,0.00003700656,0.0000046920677,0.0005523754,0.000005533312,0.0005869628],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999223,0.0000050945005,0.000004236018,0.000021746933,0.00002749943,0.000019007832],"domain_scores_gemma":[0.99971527,0.000027308386,0.00014734066,0.000025592619,0.000029059092,0.00005541386],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014375412,0.00018328828,0.00018775232,0.00069066783,0.00041826305,0.0003943998,0.00026202865,0.00033289008,0.001030064],"category_scores_gemma":[0.0003801046,0.00010632956,0.00009148048,0.0005706479,0.00032225088,0.00030368508,0.0005552517,0.00023681899,0.0003624997],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080107147,0.00017094519,0.5470276,0.00019994898,0.000088301626,0.009550347,0.0007112013,0.00069801894,0.3897547,0.0019221435,0.0012321026,0.04784369],"study_design_scores_gemma":[0.00003431035,0.00043227634,0.9442186,0.000022656508,0.00006282459,0.018116083,0.00034267336,0.0014243851,0.022448024,0.0013209824,0.011555458,0.000021767844],"about_ca_topic_score_codex":0.00030621476,"about_ca_topic_score_gemma":0.00053503364,"teacher_disagreement_score":0.001030064,"about_ca_system_score_codex":0.0001398158,"about_ca_system_score_gemma":0.00009188991,"threshold_uncertainty_score":0.0034458637},"labels":[],"label_agreement":null},{"id":"W2019317702","doi":"10.1086/320086","title":"The Inner Nebula and Central Binary of the Symbiotic Star HM Sagittae","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Nebula; Astrophysics; Extinction (optical mineralogy); Astronomy; Binary number; Planetary nebula; Line-of-sight; Stars; Optics","score_opus":0.0052509207702678504,"score_gpt":0.19655192796455426,"score_spread":0.19130100719428642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019317702","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99664766,0.00032360555,0.00023558867,0.000020297673,0.00000545498,0.0000031367288,0.0001619106,0.000037005495,0.0025653783],"genre_scores_gemma":[0.99855226,0.00005762044,0.00040504098,0.000020840758,0.000007854752,0.0000013459442,0.00052007055,0.0000051006177,0.00042983046],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993885,0.0000058539363,0.0000022424224,0.000021520265,0.000015042376,0.00001651225],"domain_scores_gemma":[0.9998411,0.000009163273,0.00004909962,0.000014285018,0.000017234486,0.0000690973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000104920386,0.00016942514,0.00023413493,0.00082955515,0.0004638561,0.00052564073,0.00023658744,0.00025387885,0.0013349139],"category_scores_gemma":[0.00019915274,0.00014630385,0.00008394432,0.00043234928,0.0002275713,0.0003299441,0.000728023,0.0001633913,0.0003402968],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032386207,0.00019759774,0.7968429,0.00008030127,0.00007980291,0.0020110225,0.0007203864,0.00068245863,0.16504082,0.00085306726,0.0013494086,0.03181826],"study_design_scores_gemma":[0.00000615601,0.00007889701,0.9942199,0.0000087938815,0.000010771398,0.0008937377,0.00009846498,0.00094648555,0.001300331,0.00016112681,0.0022698946,0.0000055029454],"about_ca_topic_score_codex":0.004020192,"about_ca_topic_score_gemma":0.008554213,"teacher_disagreement_score":0.004020192,"about_ca_system_score_codex":0.00021815594,"about_ca_system_score_gemma":0.00011285408,"threshold_uncertainty_score":0.007993579},"labels":[],"label_agreement":null},{"id":"W2019372921","doi":"10.1088/0004-637x/774/2/106","title":"A MEGACAM SURVEY OF OUTER HALO SATELLITES. II. BLUE STRAGGLERS IN THE LOWEST STELLAR DENSITY SYSTEMS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Blue straggler; Globular cluster; Milky Way; Halo; Dwarf galaxy; Stars; Stellar density; Stellar collision","score_opus":0.01240364484026323,"score_gpt":0.2077951487501389,"score_spread":0.19539150390987567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019372921","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95843494,0.0012450526,0.0004008137,0.00028983626,0.000019184366,0.00003509386,0.023611967,0.000086585875,0.015876396],"genre_scores_gemma":[0.96634775,0.0005838227,0.0023282934,0.00017360033,0.000026889144,0.00004019778,0.022548795,0.00002953919,0.007921167],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990165,0.000012825863,0.0000059853096,0.00002499327,0.000032113392,0.000022443704],"domain_scores_gemma":[0.99938214,0.000035673096,0.00015478996,0.000060832277,0.00015679002,0.00020978283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020761529,0.00008726676,0.00009922026,0.0022146746,0.0003507404,0.00029111764,0.00023190632,0.00017844529,0.0030707067],"category_scores_gemma":[0.00045330756,0.000110764435,0.00009607914,0.0018185957,0.0001152834,0.00026336484,0.00064078433,0.00017797765,0.0008705051],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009575028,0.00003038085,0.9460888,0.000054091794,0.000032143795,0.00007250829,0.0005038879,0.00014176613,0.0034853085,0.0007191716,0.009745776,0.03903033],"study_design_scores_gemma":[0.0000032690598,0.000008929874,0.9909924,0.000011048039,0.0000057590983,0.00005034169,0.0002035165,0.00010129191,0.00017791055,0.000054240714,0.0083896695,0.0000017353601],"about_ca_topic_score_codex":0.053098492,"about_ca_topic_score_gemma":0.15288714,"teacher_disagreement_score":0.053098492,"about_ca_system_score_codex":0.00041947674,"about_ca_system_score_gemma":0.00045024112,"threshold_uncertainty_score":0.10557884},"labels":[],"label_agreement":null},{"id":"W2019383013","doi":"10.1088/0004-637x/763/1/35","title":"PRECISION MEASUREMENT OF THE MOST DISTANT SPECTROSCOPICALLY CONFIRMED SUPERNOVA Ia WITH THE<i>HUBBLE SPACE TELESCOPE</i>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Quest University Canada","funders":"","keywords":"Grism; Physics; Wide Field Camera 3; Astrophysics; Redshift; Hubble space telescope; Supernova; Galaxy; Photometry (optics); Advanced Camera for Surveys; Astronomy; Observational cosmology; Hubble Deep Field; Emission spectrum; Spectral line; Stars","score_opus":0.008434829229941205,"score_gpt":0.21161134505763157,"score_spread":0.20317651582769036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019383013","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9840125,0.0017172743,0.005940486,0.00011537472,0.000040613937,0.00001714346,0.0012695609,0.00021495468,0.0066720997],"genre_scores_gemma":[0.9954324,0.00020280147,0.0033231694,0.000038425413,0.000046878547,0.0000034220052,0.0007053009,0.000010705844,0.00023702183],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99961543,0.000027969327,0.00002487022,0.00016571778,0.00011549651,0.00005042989],"domain_scores_gemma":[0.99789244,0.00024495446,0.00096660067,0.00035665385,0.00027563356,0.00026366737],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007201758,0.00030520398,0.00023053527,0.0014147453,0.0004602019,0.00080815906,0.0006245578,0.00042643625,0.0008376637],"category_scores_gemma":[0.0016787762,0.00019047598,0.00021360061,0.0005999531,0.00040680257,0.0005224486,0.0006413629,0.00041570255,0.0005426764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003017848,0.000085260515,0.8381958,0.00011014973,0.00014723817,0.00036334514,0.00018987879,0.0009805234,0.1208387,0.0011128858,0.00084039674,0.036834124],"study_design_scores_gemma":[0.00000969339,0.00012667009,0.9760297,0.000018074179,0.000067883324,0.0009529539,0.00003422169,0.00063740055,0.019208914,0.00051655894,0.0023755708,0.00002247106],"about_ca_topic_score_codex":0.0023370164,"about_ca_topic_score_gemma":0.0045107626,"teacher_disagreement_score":0.0023370164,"about_ca_system_score_codex":0.00037253433,"about_ca_system_score_gemma":0.00020169685,"threshold_uncertainty_score":0.0046468973},"labels":[],"label_agreement":null},{"id":"W2019485090","doi":"10.1088/0004-637x/773/2/84","title":"A NON-LTE ANALYSIS OF THE HOT SUBDWARF O STAR BD+28°4211. I. THE UV SPECTRUM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Subdwarf; Spectral line; Surface gravity; Effective temperature; Parallax; Calibration; Range (aeronautics); Stellar atmosphere; Opacity","score_opus":0.007654031425460181,"score_gpt":0.20875292353797809,"score_spread":0.2010988921125179,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019485090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977785,0.00007476036,0.0003516429,0.000009352611,0.0000018318395,0.0000023120563,0.0003349826,0.000023612389,0.0014230495],"genre_scores_gemma":[0.99747664,0.00005111454,0.00044894146,0.000015563135,0.000003458037,0.0000030423182,0.0015198311,0.00001579199,0.00046560477],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994826,0.0000051763227,0.0000025438096,0.000017475839,0.00001549699,0.000011066404],"domain_scores_gemma":[0.99988663,0.000018035904,0.000020167512,0.000025590658,0.000028004302,0.000021601512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007802706,0.00022878878,0.0001609405,0.00051920314,0.00026536637,0.00032518772,0.0001912897,0.00017771701,0.0008402458],"category_scores_gemma":[0.00020812567,0.00012343648,0.00024145625,0.00038234566,0.000115086696,0.0001598982,0.00029125536,0.00013101356,0.00029950868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006036417,0.00014309047,0.7583819,0.00013711712,0.00014044374,0.00067350536,0.00034951462,0.016952597,0.18318401,0.0011588869,0.00093577604,0.037339464],"study_design_scores_gemma":[0.000012801141,0.00008897599,0.9736438,0.000005886517,0.00002315082,0.00017833534,0.00012797352,0.016982429,0.00703753,0.00030265356,0.0015882029,0.000008232007],"about_ca_topic_score_codex":0.0044261836,"about_ca_topic_score_gemma":0.008411784,"teacher_disagreement_score":0.0044261836,"about_ca_system_score_codex":0.00039536937,"about_ca_system_score_gemma":0.00010848193,"threshold_uncertainty_score":0.008800864},"labels":[],"label_agreement":null},{"id":"W2019546817","doi":"10.1086/342473","title":"A Survey for Pulsating Hot B Subdwarfs in the Northern Hemisphere","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Subdwarf; Astrophysics; Stars; Light curve; Luminosity; Instability strip; Brightness; Apparent magnitude; Astronomy; White dwarf; Hertzsprung–Russell diagram; Amplitude; Stellar evolution; Galaxy; Optics","score_opus":0.027067581804183213,"score_gpt":0.23791670974591994,"score_spread":0.2108491279417367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019546817","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967253,0.00018444165,0.00026491447,0.000042216878,0.0000017407281,0.000018329494,0.0010381702,0.00003423447,0.001690512],"genre_scores_gemma":[0.99418384,0.00034490568,0.0009837191,0.00005596834,0.00001553269,0.000026115415,0.0027997973,0.000009138741,0.0015810025],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985814,0.00001872524,0.000009764229,0.000031839285,0.000044763343,0.000036684523],"domain_scores_gemma":[0.99947125,0.000041291216,0.00012128053,0.0000366633,0.000089138186,0.00024038224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029262615,0.00021533342,0.00019315092,0.0012747827,0.00046561746,0.000317765,0.0001677434,0.00015137845,0.0021789207],"category_scores_gemma":[0.000402585,0.00011895981,0.00011640273,0.0011143438,0.00015268839,0.00021985924,0.00029042378,0.00009681065,0.0005846223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006493432,0.000036521826,0.9638533,0.000029501512,0.000021153584,0.00022854982,0.0005262184,0.000059790007,0.0066850996,0.00007958802,0.0009158115,0.027499624],"study_design_scores_gemma":[0.0000037495283,0.00004015886,0.9975586,0.0000022240447,0.00000535858,0.00020221848,0.00012491582,0.000072801704,0.00022168408,0.000023737559,0.0017429471,0.0000016336716],"about_ca_topic_score_codex":0.011955239,"about_ca_topic_score_gemma":0.017897109,"teacher_disagreement_score":0.011955239,"about_ca_system_score_codex":0.00022674308,"about_ca_system_score_gemma":0.00038844143,"threshold_uncertainty_score":0.023771286},"labels":[],"label_agreement":null},{"id":"W2019578593","doi":"10.1086/323239","title":"Hydrodynamic Drag in Cosmological Simulations","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Western University","funders":"","keywords":"Physics; Drag; Supersonic speed; RADIUS; Smoothing; Smoothed-particle hydrodynamics; Mechanics; Astrophysics; Classical mechanics; Drag coefficient","score_opus":0.008945613590232456,"score_gpt":0.22752311619698248,"score_spread":0.21857750260675002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019578593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9196052,0.0012884047,0.050618753,0.0014800358,0.00018562294,0.00012612234,0.0005814128,0.000988456,0.02512603],"genre_scores_gemma":[0.98241735,0.00034729313,0.01525074,0.00011929859,0.000053302516,0.000070271344,0.00023729567,0.0002286167,0.0012759537],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99942493,0.00028806596,0.000023986056,0.00005253405,0.00013633654,0.00007419525],"domain_scores_gemma":[0.9956934,0.0028593151,0.00039712994,0.00030765127,0.00036008182,0.00038243277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013937027,0.00068415113,0.00080865744,0.0010903489,0.0012776594,0.0014731571,0.0012074847,0.001331904,0.0018977002],"category_scores_gemma":[0.011316016,0.0006674308,0.00053474336,0.0011342062,0.0012863532,0.0013896556,0.0016042887,0.001057358,0.00021262607],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000841986,0.000060719758,0.004785567,0.000057956713,0.000045648456,0.000121057295,0.00017958802,0.96342057,0.0011638136,0.025234107,0.0010079179,0.0038388204],"study_design_scores_gemma":[0.000024199186,0.000013719575,0.0005223464,0.000007426666,0.000007810963,0.000012618217,0.0000167573,0.9946138,0.0002454767,0.0039487234,0.00057695946,0.000010162905],"about_ca_topic_score_codex":0.020878844,"about_ca_topic_score_gemma":0.011655889,"teacher_disagreement_score":0.020878844,"about_ca_system_score_codex":0.0019984886,"about_ca_system_score_gemma":0.0012291202,"threshold_uncertainty_score":0.041514635},"labels":[],"label_agreement":null},{"id":"W2019595214","doi":"10.1086/505190","title":"The Ages of Elliptical Galaxies from Infrared Spectral Energy Distributions","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Astrophysics; Physics; Galaxy; Stars; Spectral energy distribution; Infrared; Luminous infrared galaxy; Stellar population; Luminosity; Spectral line; Astronomy; Equivalent width; Population; Emission spectrum; Star formation; Demography","score_opus":0.004362847843667457,"score_gpt":0.19046839019051615,"score_spread":0.1861055423468487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019595214","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911213,0.0006440353,0.0019149743,0.000026304304,0.000010663942,0.00000817834,0.0014098875,0.00006319566,0.0048014405],"genre_scores_gemma":[0.9964154,0.00024157892,0.00096515706,0.000015689144,0.000012205976,0.000008220708,0.0015185687,0.000017828215,0.0008053198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997793,0.000031282692,0.000022311257,0.000071148264,0.000049369803,0.000046640776],"domain_scores_gemma":[0.9980362,0.0004551074,0.0006355908,0.00019554651,0.00048527037,0.00019226312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077394187,0.0002269332,0.00014796581,0.0031942786,0.00016019457,0.0006530141,0.00023039598,0.00018656842,0.0011705863],"category_scores_gemma":[0.0024901824,0.00014786271,0.000248776,0.00074626965,0.00027693465,0.0005339228,0.00044504253,0.00023958473,0.00074408535],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011801335,0.000011196527,0.97222,0.000027797085,0.000048389968,0.000039155857,0.000409651,0.00090237433,0.005005628,0.0007258734,0.00039760437,0.020094194],"study_design_scores_gemma":[0.0000015245577,0.000012043861,0.9960808,0.000008063395,0.0000148230765,0.00006558111,0.000089451045,0.000555964,0.0011268632,0.0003394326,0.0016998454,0.00000560627],"about_ca_topic_score_codex":0.0021028465,"about_ca_topic_score_gemma":0.002597568,"teacher_disagreement_score":0.0031942786,"about_ca_system_score_codex":0.00042226046,"about_ca_system_score_gemma":0.00009200678,"threshold_uncertainty_score":0.004181206},"labels":[],"label_agreement":null},{"id":"W2019607503","doi":"10.1086/338926","title":"Infrared Absorption and Emission Spectra of Hydrogenated Amorphous Carbon Prepared in the Presence of Oxygen, Nitrogen, Ammonia, and Carbon Monoxide","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Diamond and Carbon-based Materials Research","field":"Materials Science","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Oxygen; Amorphous carbon; Carbon fibers; Absorption (acoustics); Absorption spectroscopy; Carbon monoxide; Analytical Chemistry (journal); Amorphous solid; Nitrogen; Infrared spectroscopy; Spectral line; Graphite; Infrared; Chemistry; Materials science; Physics; Organic chemistry; Optics","score_opus":0.011709818422496503,"score_gpt":0.22746761297599338,"score_spread":0.2157577945534969,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019607503","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978765,0.00022923603,0.00060655514,0.000015224265,0.0000061285164,0.0000077970835,0.00017472253,0.000015489992,0.0010682759],"genre_scores_gemma":[0.9975867,0.00018461267,0.0010652879,0.000017935925,0.000004387514,0.0000130651,0.0003780238,0.00001081734,0.0007391168],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99987376,0.00001673685,0.0000068741374,0.000026200183,0.00004954394,0.000026742811],"domain_scores_gemma":[0.99975294,0.000100415964,0.000043799344,0.000021910295,0.00005072766,0.000030126024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018265478,0.00026517746,0.00013102418,0.00035884386,0.00028705408,0.00016171239,0.00028670998,0.00036222127,0.001089784],"category_scores_gemma":[0.000250355,0.00010673957,0.00010519338,0.0003508494,0.00027788655,0.00014585185,0.00008538769,0.0002915946,0.00010391346],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009279987,0.00001794099,0.00024764717,0.000018040122,0.000005281582,0.00004176253,0.000021315615,0.00012208881,0.9989177,0.000038465892,0.000012780059,0.0004642508],"study_design_scores_gemma":[0.000011243682,0.00019379998,0.0077802874,0.0000057251364,0.000007320787,0.0000488578,0.000037532594,0.0008185572,0.9906921,0.000022830547,0.00037565202,0.0000060226903],"about_ca_topic_score_codex":0.001912551,"about_ca_topic_score_gemma":0.0017629721,"teacher_disagreement_score":0.001912551,"about_ca_system_score_codex":0.00022387203,"about_ca_system_score_gemma":0.00011926092,"threshold_uncertainty_score":0.0038027763},"labels":[],"label_agreement":null},{"id":"W2019634125","doi":"10.1088/0004-637x/778/1/74","title":"WEAK LENSING CALIBRATED<i>M</i>-<i>T</i>SCALING RELATION OF GALAXY GROUPS IN THE COSMOS FIELD","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Magnus Ehrnroothin Säätiö; Centre National de la Recherche Scientifique; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Associated Universities; California Institute of Technology; National Aeronautics and Space Administration; Academy of Finland; National Radio Astronomy Observatory; European Southern Observatory; National Science Foundation","keywords":"Physics; Weak gravitational lensing; Astrophysics; Cosmology; Galaxy cluster; Redshift; Hydrostatic equilibrium; Galaxy; Scaling; Observable; Cluster (spacecraft); Astronomy","score_opus":0.007997575583396477,"score_gpt":0.20317421592382115,"score_spread":0.19517664034042467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019634125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99543095,0.00013104547,0.001963281,0.000021131178,0.0000036675472,0.0000075859384,0.0003059407,0.000052463165,0.002083961],"genre_scores_gemma":[0.99890876,0.000030577226,0.0006296316,0.00000833988,0.000006259322,0.0000035544108,0.00032373494,0.00001177036,0.00007727135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995703,0.00008528342,0.000026358191,0.00020103331,0.000071142626,0.000045926998],"domain_scores_gemma":[0.9971819,0.00055932585,0.0011926504,0.0006491729,0.00024649999,0.00017045888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008175806,0.0003874813,0.0002188856,0.0016664158,0.00025522703,0.0006639109,0.0002486247,0.00018326397,0.0010941473],"category_scores_gemma":[0.004113844,0.00020289273,0.00023366616,0.0010651742,0.0005732354,0.0004902694,0.00067166594,0.00025162927,0.00033673042],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008269556,0.000026540913,0.9733889,0.0000301624,0.00007430306,0.000048146776,0.00018464943,0.0021446918,0.010234552,0.001352208,0.0003479545,0.012085165],"study_design_scores_gemma":[0.0000062267345,0.000031498832,0.9881995,0.000007483449,0.000025628993,0.00008810441,0.000053389125,0.005094451,0.004638794,0.0011357039,0.0007108093,0.000008432657],"about_ca_topic_score_codex":0.0022868195,"about_ca_topic_score_gemma":0.0016518625,"teacher_disagreement_score":0.0022868195,"about_ca_system_score_codex":0.00043834612,"about_ca_system_score_gemma":0.00012932402,"threshold_uncertainty_score":0.0045469403},"labels":[],"label_agreement":null},{"id":"W2019692459","doi":"10.1086/524402","title":"Searching for Non-Gaussian Signals in the BOOMERANG 2003 CMB Maps","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Gaussian; Estimator; Minkowski space; Non-Gaussianity; Amplitude; Parameter space; Cosmic background radiation; Astrophysics; Statistical physics; Statistics; Optics; Mathematical physics; Quantum mechanics","score_opus":0.011042367792554278,"score_gpt":0.28742745041624157,"score_spread":0.2763850826236873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019692459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99098396,0.000081201244,0.0068550156,0.0000703316,0.000002151601,0.00000910574,0.0002635689,0.0001397639,0.0015949701],"genre_scores_gemma":[0.9972504,0.00001846086,0.0022319693,0.000017077446,0.0000023394014,0.00000583666,0.0003512886,0.00003041621,0.00009212982],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996754,0.00009601312,0.000010138458,0.00008143673,0.000058607577,0.00007843705],"domain_scores_gemma":[0.99863166,0.0005518468,0.00030060526,0.00021247222,0.00015024997,0.00015312705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012190081,0.00031029026,0.00027385063,0.0012224556,0.0005577573,0.00089321705,0.00043279974,0.00027358913,0.0009399139],"category_scores_gemma":[0.0032109881,0.0002693841,0.0003386734,0.00093544053,0.0005646104,0.00027750555,0.0005893992,0.00029244737,0.00016898145],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011332112,0.00010928203,0.83946306,0.00013107141,0.00037112136,0.0005556319,0.0015907639,0.03704323,0.054787487,0.022820976,0.001844606,0.04014961],"study_design_scores_gemma":[0.00003593778,0.000049842067,0.90032953,0.000019652449,0.000067212866,0.00021821502,0.00017575304,0.08001886,0.01106398,0.0046118805,0.003358033,0.000051003164],"about_ca_topic_score_codex":0.009766346,"about_ca_topic_score_gemma":0.015106084,"teacher_disagreement_score":0.009766346,"about_ca_system_score_codex":0.0005869763,"about_ca_system_score_gemma":0.00030375028,"threshold_uncertainty_score":0.019419014},"labels":[],"label_agreement":null},{"id":"W2019744752","doi":"10.1086/312693","title":"Diffusion in the Atmospheres of Blue Horizontal-Branch Stars","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Moncton","funders":"","keywords":"Physics; Diffusion; Horizontal branch; Atmosphere (unit); Stars; Stellar atmosphere; Astrophysics; Magnitude (astronomy); Diagram; Meteorology; Thermodynamics; Metallicity","score_opus":0.006881333262051504,"score_gpt":0.21155518110334257,"score_spread":0.20467384784129106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019744752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974969,0.00009305622,0.001676986,0.00007502592,0.0000046456194,0.000004842742,0.00005910012,0.000058127065,0.0005313495],"genre_scores_gemma":[0.9989894,0.00007736791,0.00069970987,0.000010967759,0.000005653002,0.000004085665,0.00006874464,0.000018907713,0.00012517149],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998846,0.000040166713,0.000006793095,0.000024313415,0.000016931046,0.000027216442],"domain_scores_gemma":[0.99930525,0.00027083248,0.00015203572,0.00005579816,0.00008995173,0.00012614268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002984099,0.0005900127,0.00039223072,0.00034070437,0.0005704543,0.0006539916,0.0005768382,0.00060770713,0.00044578896],"category_scores_gemma":[0.0017144221,0.00042530886,0.00056523934,0.00035335537,0.00055762276,0.0010850235,0.0009522285,0.00044304106,0.00009465973],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032465297,0.0001466725,0.095377035,0.000091716865,0.00015449592,0.00036958902,0.00050380913,0.8410894,0.048508704,0.008723155,0.00040616468,0.004304607],"study_design_scores_gemma":[0.00009512151,0.000060085888,0.012948893,0.000004965536,0.000028540999,0.00004977743,0.00004246813,0.9820374,0.0030225995,0.0014507556,0.0002361906,0.000023158393],"about_ca_topic_score_codex":0.01834058,"about_ca_topic_score_gemma":0.0064118695,"teacher_disagreement_score":0.01834058,"about_ca_system_score_codex":0.0010470259,"about_ca_system_score_gemma":0.00050211675,"threshold_uncertainty_score":0.03646767},"labels":[],"label_agreement":null},{"id":"W2019789687","doi":"10.1086/320679","title":"High-Latitude Galactic Dust Emission in the BOOMERANG Maps","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Brightness temperature; Astronomy; Microwave; Brightness; Cosmic dust; Latitude; Optics","score_opus":0.011594864651640181,"score_gpt":0.2449810147123733,"score_spread":0.23338615006073313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019789687","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99222624,0.00011622765,0.0005420887,0.00007833853,0.0000036407582,0.0000034626705,0.00097369,0.00006204611,0.005994221],"genre_scores_gemma":[0.99772483,0.00006299673,0.00052160106,0.000016956117,0.0000044715466,0.0000031417635,0.0010587252,0.00001957843,0.0005876723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998727,0.000017390928,0.0000021626015,0.00003509364,0.000021437278,0.000051182873],"domain_scores_gemma":[0.9997979,0.000028540519,0.00006472359,0.000038828206,0.00002874007,0.000041273208],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014284751,0.00019711096,0.00015603888,0.0009394214,0.00040651322,0.00061619765,0.00012480216,0.00012962069,0.0012251543],"category_scores_gemma":[0.0002840247,0.0001562208,0.00014487689,0.0010053378,0.0003686694,0.0001929271,0.00043881542,0.00020368783,0.00026876968],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012663733,0.00011108915,0.86565524,0.00012002807,0.0002246889,0.0008796113,0.0020713245,0.0051446646,0.06298263,0.007472779,0.005850722,0.048220944],"study_design_scores_gemma":[0.000008533407,0.000014387201,0.99142563,0.000006424397,0.00001990359,0.00013868939,0.00008782219,0.0009810376,0.001753061,0.0002606161,0.005290119,0.000013693451],"about_ca_topic_score_codex":0.021784712,"about_ca_topic_score_gemma":0.075190604,"teacher_disagreement_score":0.021784712,"about_ca_system_score_codex":0.00048389792,"about_ca_system_score_gemma":0.00011962481,"threshold_uncertainty_score":0.043315828},"labels":[],"label_agreement":null},{"id":"W2019992772","doi":"10.1088/0004-637x/802/1/46","title":"<i>MC</i><sup>2</sup>: CONSTRAINING THE DARK MATTER DISTRIBUTION OF THE VIOLENT MERGING GALAXY CLUSTER CIZA J2242.8+5301 BY PIERCING THROUGH THE MILKY WAY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Lawrence Livermore National Laboratory; Smithsonian Institution; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; Fundação para a Ciência e a Tecnologia; Smithsonian Astrophysical Observatory; U.S. Department of Energy","keywords":"Physics; Dark matter; Astrophysics; Galaxy cluster; Galaxy; Cluster (spacecraft); Milky Way; Dark matter halo; Mass distribution; Halo; Satellite galaxy; Astronomy; Computer science","score_opus":0.009185540398028845,"score_gpt":0.21487151313332492,"score_spread":0.20568597273529607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2019992772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9838346,0.00018998551,0.004936615,0.00033315032,0.000027960425,0.000025235146,0.003034685,0.0004724126,0.007145299],"genre_scores_gemma":[0.99440044,0.00005404254,0.0026835059,0.00006223415,0.000023838262,0.000020677156,0.0022088436,0.000092456285,0.00045396484],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990857,0.00002011281,0.000004502556,0.000018319733,0.000029233785,0.000019241223],"domain_scores_gemma":[0.9991379,0.00039501855,0.00014078575,0.00010960432,0.0000930159,0.00012371955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028858308,0.00030546714,0.00027653994,0.00042065,0.00041617046,0.0009645195,0.000813391,0.00036729148,0.0038305416],"category_scores_gemma":[0.0024330262,0.00020740654,0.00034884212,0.00031249633,0.00034718393,0.0002202478,0.0004594,0.0003091758,0.0005094762],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013759483,0.00009812274,0.4847119,0.00019038477,0.00040589142,0.0011314115,0.00024720287,0.4207833,0.044724066,0.00871328,0.013368028,0.02425052],"study_design_scores_gemma":[0.00008796754,0.0001294184,0.42664027,0.000051119165,0.00016249108,0.00039703114,0.00024821132,0.5429949,0.019659191,0.003569481,0.005972801,0.00008715081],"about_ca_topic_score_codex":0.021678308,"about_ca_topic_score_gemma":0.025596688,"teacher_disagreement_score":0.021678308,"about_ca_system_score_codex":0.00072707736,"about_ca_system_score_gemma":0.00038379527,"threshold_uncertainty_score":0.04310423},"labels":[],"label_agreement":null},{"id":"W2020060144","doi":"10.1086/427551","title":"The Dearth of Massive, Helium-rich White Dwarfs in Young Open Star Clusters","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Open cluster; Helium; White dwarf; Astrophysics; Cluster (spacecraft); Star cluster; Stellar classification; Population; Spectral line; Hydrogen; Astronomy; Stars; Atomic physics; Medicine","score_opus":0.01002155464617269,"score_gpt":0.23329270423053206,"score_spread":0.22327114958435937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020060144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993437,0.00016190638,0.00011570982,0.000011764003,0.00000202095,9.154753e-7,0.00011064213,0.0000054872603,0.00024776414],"genre_scores_gemma":[0.99918,0.0001534413,0.00013014497,0.000020507421,0.000006700692,0.0000018195435,0.0002816141,0.000003062521,0.00022273899],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996785,0.00002572116,0.000047772075,0.000109427936,0.0000914132,0.000047185404],"domain_scores_gemma":[0.9983564,0.00038934674,0.0006283821,0.00022958108,0.0001541289,0.0002421772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040521438,0.00014466084,0.00029772872,0.0013551184,0.00071509066,0.00087494147,0.00031691333,0.00033906847,0.00048641395],"category_scores_gemma":[0.0016764586,0.00019228432,0.00012325805,0.00093689543,0.00063500996,0.00045856964,0.0005912421,0.00018638333,0.00019120218],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025793086,0.000029621357,0.9572969,0.00006243653,0.000047877413,0.00053729827,0.0008075162,0.00016986551,0.029995408,0.0003531059,0.00018993253,0.010252133],"study_design_scores_gemma":[0.0000022626853,0.00002759798,0.9965503,0.0000053674985,0.000013617504,0.0005145219,0.0001781208,0.00007291014,0.0018925822,0.000119881304,0.00061766454,0.0000052138557],"about_ca_topic_score_codex":0.0021680994,"about_ca_topic_score_gemma":0.00397104,"teacher_disagreement_score":0.0021680994,"about_ca_system_score_codex":0.00025346768,"about_ca_system_score_gemma":0.00016533653,"threshold_uncertainty_score":0.004311025},"labels":[],"label_agreement":null},{"id":"W2020282587","doi":"10.1086/507320","title":"The Burst Mode of Protostellar Accretion","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":378,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Protostar; Astrophysics; Physics; Accretion (finance); Angular momentum; Protoplanetary disk; Astronomy; Burst mode (computing); Star formation; Gravitational instability; Planet; Stars","score_opus":0.00657295746625695,"score_gpt":0.23474420699167498,"score_spread":0.22817124952541804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020282587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98386097,0.0000948543,0.008804595,0.0001242595,0.000028696057,0.00003326186,0.00020966762,0.00010917445,0.0067344164],"genre_scores_gemma":[0.99570966,0.000062284,0.0031193052,0.00004237815,0.000006888666,0.00002859985,0.00019291932,0.000031373365,0.00080659316],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999138,0.000016911143,0.0000037545335,0.000015443124,0.000017901017,0.00003219968],"domain_scores_gemma":[0.99955684,0.00015306646,0.00008292497,0.000045855308,0.00007453229,0.00008684448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002507066,0.00034224073,0.00047250048,0.00025468835,0.0004229854,0.00066760107,0.0009331137,0.0007124416,0.0012916859],"category_scores_gemma":[0.001767872,0.00020281092,0.0003732791,0.0002827408,0.00061440695,0.0006250002,0.0004434718,0.0006972582,0.00014942934],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011603325,0.00008479763,0.0080270665,0.000033797853,0.000036611866,0.00019377192,0.000114493574,0.9811404,0.0032786946,0.0044629145,0.00047878784,0.0020326588],"study_design_scores_gemma":[0.000018438612,0.000015120698,0.00063570275,0.0000025926654,0.000003907002,0.000013313145,0.00001901871,0.9982957,0.00034505746,0.00047118045,0.00017671626,0.0000032535006],"about_ca_topic_score_codex":0.015806904,"about_ca_topic_score_gemma":0.0070514153,"teacher_disagreement_score":0.015806904,"about_ca_system_score_codex":0.00067023106,"about_ca_system_score_gemma":0.0006871501,"threshold_uncertainty_score":0.031429827},"labels":[],"label_agreement":null},{"id":"W2020295154","doi":"10.1086/505792","title":"Differential Rotation of ε Eridani Detected by<i>MOST</i>","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Saint Mary's University; University of Victoria; University of Toronto; St. Mary's University; Dominion Astrophysical Observatory; University of British Columbia","funders":"","keywords":"Physics; Differential rotation; Rotation (mathematics); Astrophysics; Astronomy; Differential (mechanical device); Stellar rotation; Stars; Geometry","score_opus":0.00472926887414827,"score_gpt":0.194843789403539,"score_spread":0.19011452052939073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020295154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99430734,0.0001123903,0.0006727661,0.000035277528,0.0000067491183,0.000002650123,0.00044340236,0.000054182332,0.0043651885],"genre_scores_gemma":[0.99797934,0.000035120505,0.00067706977,0.000020128966,0.0000040133077,0.0000028852514,0.0005631564,0.000018606435,0.000699608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983466,0.000013436566,0.0000115222065,0.0000736744,0.000032890894,0.000033729437],"domain_scores_gemma":[0.9997532,0.000015674184,0.0001002235,0.00003433729,0.000055614233,0.000040914158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023666437,0.00018332146,0.00014777927,0.00053532363,0.00022668863,0.00046532636,0.00030669244,0.00022313219,0.001430472],"category_scores_gemma":[0.00040879162,0.00013677357,0.00013416966,0.00042313262,0.00014347956,0.00024921828,0.00045981188,0.00021558076,0.00051960687],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044043438,0.000041341944,0.6759017,0.00008231163,0.0000619287,0.0003038839,0.0006164977,0.000773853,0.2816492,0.00090884435,0.001486863,0.03773316],"study_design_scores_gemma":[0.0000034914094,0.00003726799,0.9663975,0.000007340344,0.000014806988,0.00023122938,0.00010753452,0.0010251353,0.027478937,0.00009087636,0.0045976313,0.000008237495],"about_ca_topic_score_codex":0.0018955644,"about_ca_topic_score_gemma":0.0028971375,"teacher_disagreement_score":0.0018955644,"about_ca_system_score_codex":0.0004002324,"about_ca_system_score_gemma":0.00008284782,"threshold_uncertainty_score":0.0047854185},"labels":[],"label_agreement":null},{"id":"W2020336398","doi":"10.1088/0004-637x/770/1/39","title":"THE BOLOCAM GALACTIC PLANE SURVEY. VIII. A MID-INFRARED KINEMATIC DISTANCE DISCRIMINATION METHOD","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Galactic plane; Molecular cloud; Kinematics; Galaxy; Radiative transfer; Milky Way; Stars; Millimeter; Galactic Center","score_opus":0.013996169573764912,"score_gpt":0.2668782944765742,"score_spread":0.25288212490280926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020336398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.42819118,0.0054513332,0.34578782,0.0009827575,0.0002534217,0.0005691606,0.16188848,0.007824481,0.049051266],"genre_scores_gemma":[0.5950506,0.0013515983,0.27160266,0.00023036532,0.000177386,0.00044485118,0.11698437,0.0004963464,0.013661785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996965,0.0000392675,0.000018375858,0.00009781806,0.000111616646,0.000036468446],"domain_scores_gemma":[0.9996567,0.0000229658,0.00012651397,0.00006746234,0.00009286277,0.000033561217],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004013823,0.0004368605,0.0002528657,0.0026576815,0.00025788814,0.0008006228,0.00054746127,0.0002894632,0.0026445126],"category_scores_gemma":[0.0013933411,0.00020774163,0.00035295272,0.0016212951,0.000104827384,0.00037165216,0.0006093976,0.00038886044,0.0024980523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016028827,0.000064557215,0.52645975,0.00019678035,0.00025431172,0.00018257985,0.00022693518,0.010602317,0.009691025,0.009049317,0.042593993,0.40051812],"study_design_scores_gemma":[0.00005760833,0.00003855399,0.76527387,0.000121434095,0.00006201632,0.00036661376,0.00018554638,0.03975266,0.006000353,0.0047372454,0.18337007,0.000033974622],"about_ca_topic_score_codex":0.0289219,"about_ca_topic_score_gemma":0.026003554,"teacher_disagreement_score":0.0289219,"about_ca_system_score_codex":0.0009880263,"about_ca_system_score_gemma":0.000563403,"threshold_uncertainty_score":0.057507098},"labels":[],"label_agreement":null},{"id":"W2020360271","doi":"10.1088/0004-637x/799/2/142","title":"CALIBRATION OF THE MIXING-LENGTH THEORY FOR CONVECTIVE WHITE DWARF ENVELOPES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Convection zone; Convective mixing; Convection; Physics; White dwarf; Mixing length model; Effective temperature; Astrophysics; Photosphere; Convective inhibition; Mixing (physics); Mechanics; Stars; Combined forced and natural convection; Natural convection; Astronomy; Spectral line","score_opus":0.016170704574249854,"score_gpt":0.23120272692194122,"score_spread":0.21503202234769137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020360271","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8420228,0.00042247816,0.15262492,0.0001448204,0.000045083547,0.00005924007,0.00028831325,0.00045328707,0.0039390735],"genre_scores_gemma":[0.98972815,0.00008168461,0.009794122,0.00001467904,0.000008393766,0.000043739845,0.00012929455,0.00005795052,0.00014195124],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99979645,0.000059402795,0.000014196187,0.000047202127,0.00005510899,0.00002768674],"domain_scores_gemma":[0.9994018,0.00024232909,0.00009261872,0.00014623732,0.000069045476,0.000047947695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008725301,0.0005252155,0.0002943057,0.000478674,0.00030966432,0.00065848656,0.00080852566,0.00049148593,0.0003779671],"category_scores_gemma":[0.00300488,0.00020396242,0.00046213547,0.00030348625,0.00043382644,0.00060675427,0.0008819237,0.00080018,0.00014082668],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014212177,0.00006587873,0.026101707,0.0000608835,0.00005736929,0.000112976144,0.00012142739,0.90713483,0.032555286,0.016757768,0.00020519336,0.016684517],"study_design_scores_gemma":[0.000013230351,0.00003548224,0.0048187557,0.00000879127,0.0000065311856,0.000021545526,0.000011539189,0.98206115,0.009050095,0.0036293073,0.00033034317,0.000013242343],"about_ca_topic_score_codex":0.0015835448,"about_ca_topic_score_gemma":0.0006053621,"teacher_disagreement_score":0.0015835448,"about_ca_system_score_codex":0.0009872364,"about_ca_system_score_gemma":0.00031751787,"threshold_uncertainty_score":0.0071629286},"labels":[],"label_agreement":null},{"id":"W2020406352","doi":"10.1088/0004-637x/784/1/78","title":"MASSIVE MOLECULAR GAS FLOWS IN THE A1664 BRIGHTEST CLUSTER GALAXY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Science Council; Canadian Space Agency; National Radio Astronomy Observatory; National Science Foundation","keywords":"Galaxy; Outflow; RADIUS; Galaxy cluster; Star formation; Velocity dispersion; Radial velocity; Cluster (spacecraft); Surface brightness; Line-of-sight","score_opus":0.004465924271686827,"score_gpt":0.19828239197983352,"score_spread":0.1938164677081467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020406352","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99957293,0.000038423528,0.00004005116,0.000013262453,0.0000024953035,0.0000014601356,0.000027209308,0.000011862461,0.0002922443],"genre_scores_gemma":[0.99937516,0.000021045453,0.00028465907,0.000014493367,0.000008890519,0.0000014795476,0.00009881398,0.0000029964567,0.00019234855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999131,0.000008362903,0.0000046994296,0.000024288847,0.000024503217,0.000025008194],"domain_scores_gemma":[0.99977976,0.0000147015335,0.000073939,0.000012569421,0.000021571164,0.00009750925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012924081,0.00023480202,0.00022051719,0.00082580623,0.0006696424,0.00052614644,0.00032191954,0.00035415922,0.000801935],"category_scores_gemma":[0.00033527947,0.00019932467,0.00012441681,0.00029240473,0.00032915268,0.00027295132,0.00055718824,0.00021184374,0.0002199257],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049370254,0.0001713258,0.8099484,0.000057422425,0.000065867294,0.0013399132,0.00081342,0.001260332,0.17242858,0.0005560734,0.0006694853,0.012195449],"study_design_scores_gemma":[0.00002416833,0.00018970546,0.99074006,0.0000063220136,0.000026598604,0.000553852,0.0002847471,0.002087207,0.0044784346,0.00025204688,0.0013401208,0.000016739667],"about_ca_topic_score_codex":0.0049987184,"about_ca_topic_score_gemma":0.0072113858,"teacher_disagreement_score":0.0049987184,"about_ca_system_score_codex":0.00055266486,"about_ca_system_score_gemma":0.00018950173,"threshold_uncertainty_score":0.009939253},"labels":[],"label_agreement":null},{"id":"W2020460381","doi":"10.1088/0004-637x/758/2/75","title":"ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. II. DECONSTRUCTING THE THERMAL SZ POWER SPECTRUM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":215,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Intracluster medium; Cosmic microwave background; Galaxy cluster; Spectral density; RADIUS; Cluster (spacecraft); Redshift; Sunyaev–Zel'dovich effect; Galaxy; Substructure; Computational physics; Anisotropy; Optics","score_opus":0.008196285523402244,"score_gpt":0.207924869574368,"score_spread":0.19972858405096577,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020460381","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94060415,0.0020705368,0.026228687,0.0017052836,0.00006104642,0.00006515882,0.000934445,0.00018578563,0.028144972],"genre_scores_gemma":[0.99387336,0.0006685406,0.0037443729,0.00011732363,0.00003758549,0.000024244742,0.00026523406,0.00005030924,0.00121914],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984825,0.000049206337,0.000003824757,0.000027829885,0.000038716054,0.000032096705],"domain_scores_gemma":[0.999539,0.00020064262,0.00011388418,0.000048546997,0.000045049866,0.000052920117],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068546424,0.00022942838,0.0002239429,0.0011766606,0.00042392878,0.00079747394,0.00046440467,0.000254854,0.0015374911],"category_scores_gemma":[0.002150718,0.00020251815,0.00028893462,0.001117245,0.00069253775,0.00067998964,0.0009293986,0.00036469678,0.000120813114],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012454312,0.000034006818,0.5920989,0.00017789876,0.00021781476,0.0004977152,0.0010765356,0.10254888,0.0048125265,0.236246,0.005794285,0.05637094],"study_design_scores_gemma":[0.000023600105,0.000050115035,0.83681786,0.00007941212,0.000031232932,0.00020655298,0.00047629623,0.11098999,0.001486043,0.037058525,0.012736288,0.000044021766],"about_ca_topic_score_codex":0.01870857,"about_ca_topic_score_gemma":0.023085855,"teacher_disagreement_score":0.01870857,"about_ca_system_score_codex":0.0010957061,"about_ca_system_score_gemma":0.00042177847,"threshold_uncertainty_score":0.03719932},"labels":[],"label_agreement":null},{"id":"W2020537781","doi":"10.1086/588420","title":"Cooling of Young Stars Growing by Disk Accretion","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Research Canada; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Brown dwarf; Stars; Planet; Astronomy; Accretion (finance); Hot Jupiter; Exoplanet; Young stellar object; T Tauri star; Star formation","score_opus":0.010434444537825778,"score_gpt":0.22810415485062915,"score_spread":0.21766971031280338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020537781","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941907,0.0012620605,0.0015458127,0.000016336973,0.000008018247,0.000015251874,0.00013525593,0.000026586398,0.002799926],"genre_scores_gemma":[0.99617803,0.0006296194,0.00056970184,0.000015197134,0.000010204897,0.0000125670185,0.00023390932,0.000014671052,0.0023361451],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994683,0.000008040986,0.0000030333792,0.00001794841,0.000008042919,0.000016159558],"domain_scores_gemma":[0.99988747,0.000021867336,0.00003601792,0.000015242062,0.000015094988,0.000024226412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012967459,0.00021253283,0.00027227605,0.0001678871,0.0002827338,0.0005163284,0.00023967246,0.00023776923,0.0012773935],"category_scores_gemma":[0.0003356079,0.00011055508,0.00021349595,0.00015557995,0.00020400074,0.00019536205,0.00031182196,0.00012504075,0.0005328869],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000563398,0.00016820784,0.1748131,0.00040985536,0.000083086314,0.0010193107,0.0004884027,0.014382813,0.7640531,0.0036310132,0.0006520963,0.039735515],"study_design_scores_gemma":[0.00007650863,0.00118554,0.7663089,0.000063662286,0.00010562875,0.0029399623,0.00040647126,0.046839587,0.15797469,0.006004316,0.018060384,0.000034280925],"about_ca_topic_score_codex":0.0009961359,"about_ca_topic_score_gemma":0.00069814426,"teacher_disagreement_score":0.0012773935,"about_ca_system_score_codex":0.00031847952,"about_ca_system_score_gemma":0.00016097749,"threshold_uncertainty_score":0.0042732954},"labels":[],"label_agreement":null},{"id":"W2020609075","doi":"10.1088/0004-637x/751/2/141","title":"THE ELM SURVEY. IV. 24 WHITE DWARF MERGER SYSTEMS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"White dwarf; Gravitational wave; Supernova; Radial velocity; Sky; Interferometry","score_opus":0.01788212083144345,"score_gpt":0.23721319935700533,"score_spread":0.21933107852556188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020609075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90873766,0.0016592458,0.0008800376,0.00028883142,0.000028115743,0.00012094363,0.07382763,0.00033475837,0.014122729],"genre_scores_gemma":[0.8149838,0.0010485445,0.0031739173,0.0002843227,0.000103590064,0.00021377092,0.16523784,0.00007259441,0.014881605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997154,0.000039997398,0.000025311638,0.000057020752,0.000085735046,0.00007663488],"domain_scores_gemma":[0.99948907,0.000028672835,0.00021792341,0.00004299986,0.000073288094,0.00014801552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004574175,0.00035264564,0.00023953791,0.0030872168,0.00030939668,0.00043136478,0.00033510372,0.00018442514,0.003383246],"category_scores_gemma":[0.00043738217,0.0001407982,0.00017411598,0.001996252,0.00010471938,0.0003649966,0.00095956126,0.00016408248,0.0020941016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002123576,0.000071573464,0.9055461,0.0001846535,0.000103422804,0.00042168703,0.00045361687,0.00020386155,0.0046285354,0.0005649597,0.03455427,0.053054936],"study_design_scores_gemma":[0.000027068883,0.00004350048,0.94816744,0.000025234918,0.000020917769,0.0003195612,0.00018653568,0.00025226508,0.0007319532,0.00008197381,0.05013764,0.0000059165864],"about_ca_topic_score_codex":0.006771736,"about_ca_topic_score_gemma":0.015514437,"teacher_disagreement_score":0.006771736,"about_ca_system_score_codex":0.00040815538,"about_ca_system_score_gemma":0.00028530322,"threshold_uncertainty_score":0.01346463},"labels":[],"label_agreement":null},{"id":"W2020634432","doi":"10.1088/0004-637x/738/1/105","title":"A RADIO PULSAR SEARCH OF THE γ-RAY BINARIES LS I +61 303 AND LS 5039","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Earth Systems and Cosmic Evolution","field":"Earth and Planetary Sciences","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Pulsar; Flux (metallurgy); Compact star; Null (SQL); Star (game theory); Neutron star","score_opus":0.021156392536837626,"score_gpt":0.1982484031477353,"score_spread":0.1770920106108977,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020634432","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967069,0.00008408374,0.00021089235,0.000043527776,0.0000031785269,0.000008793092,0.00012151936,0.000016288768,0.0028048449],"genre_scores_gemma":[0.99870884,0.00004208662,0.00053993694,0.000037263253,0.0000048691436,0.0000047159797,0.0002283905,0.0000018519966,0.0004319722],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994755,0.0000066750463,0.000003863471,0.000016697479,0.000011755809,0.00001340818],"domain_scores_gemma":[0.9998311,0.000024387398,0.000047786707,0.000012914037,0.000017753568,0.00006599435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015544205,0.00015933522,0.0001780323,0.0007012205,0.00049330347,0.0004497566,0.0001703634,0.0002471867,0.0019683656],"category_scores_gemma":[0.00028228827,0.00008915783,0.00009443596,0.0005065722,0.00022069641,0.0001971418,0.00038786806,0.00014150834,0.0004610375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007584156,0.00009018307,0.8546437,0.00005251771,0.000059240258,0.002075477,0.00062138675,0.000670819,0.10736334,0.0017510838,0.00092804653,0.030985847],"study_design_scores_gemma":[0.000040059986,0.00037320456,0.9841389,0.000018631883,0.000049154805,0.0019503357,0.00065781164,0.0018914086,0.007548569,0.00063967984,0.0026783752,0.000013885298],"about_ca_topic_score_codex":0.0027381345,"about_ca_topic_score_gemma":0.0044804723,"teacher_disagreement_score":0.0027381345,"about_ca_system_score_codex":0.00020008079,"about_ca_system_score_gemma":0.00022756742,"threshold_uncertainty_score":0.006584823},"labels":[],"label_agreement":null},{"id":"W2020670657","doi":"10.1088/0004-637x/749/2/152","title":"A UNIFORM ASTEROSEISMIC ANALYSIS OF 22 SOLAR-TYPE STARS OBSERVED BY<i>KEPLER</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":198,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency","funders":"Science and Technology Facilities Council","keywords":"Asteroseismology; Oscillation (cell signaling); Stars; RADIUS; Exoplanet; Spitzer Space Telescope; Stellar mass; Sample (material); Stellar structure","score_opus":0.02008111315695379,"score_gpt":0.2306313224223336,"score_spread":0.21055020926537982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020670657","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98089314,0.000102682745,0.013862093,0.000022869464,0.000005741292,0.000051799074,0.0025954368,0.0007294586,0.0017368307],"genre_scores_gemma":[0.9606666,0.00007229325,0.02502115,0.00003236628,0.00001261599,0.00006404889,0.013384123,0.00020343321,0.0005432965],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960023,0.000058999747,0.00003564442,0.0001757335,0.000088005414,0.000041323023],"domain_scores_gemma":[0.9989304,0.00013225524,0.00024161632,0.00039308288,0.00018326483,0.00011932028],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006202633,0.0004058664,0.0004005956,0.0017284203,0.0005478768,0.0005615769,0.0004024672,0.00028735033,0.0008890087],"category_scores_gemma":[0.0014666407,0.0002246028,0.00055980857,0.0017677483,0.00020763627,0.00042032872,0.00095766754,0.00028378892,0.00060941675],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051539514,0.00035635818,0.75928825,0.00010747649,0.0002828233,0.00030915515,0.0006089155,0.024589762,0.07892449,0.00048780045,0.0028869074,0.13164261],"study_design_scores_gemma":[0.000056893543,0.00025093034,0.9328269,0.000010982472,0.00006447934,0.0003911922,0.00020609947,0.041393317,0.018737711,0.00041447202,0.0056163454,0.000030744643],"about_ca_topic_score_codex":0.0037392802,"about_ca_topic_score_gemma":0.0058989883,"teacher_disagreement_score":0.0037392802,"about_ca_system_score_codex":0.00026822725,"about_ca_system_score_gemma":0.00032888452,"threshold_uncertainty_score":0.007435024},"labels":[],"label_agreement":null},{"id":"W2020693322","doi":"10.1086/421838","title":"Quasi‐periodic Inward Shock Formations in the System of a Black Hole and an Accretion Disk and Application to Quasi‐periodic Oscillations in Galactic Black Hole Candidates","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Perturbation (astronomy); Shock wave; Astrophysics; Kerr metric; Black hole (networking); Oscillation (cell signaling); Rotating black hole; Accretion (finance); Classical mechanics; Mechanics; Astronomy; Schwarzschild radius","score_opus":0.009575400899046151,"score_gpt":0.24514612409100744,"score_spread":0.2355707231919613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020693322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99546045,0.000052670064,0.0032711388,0.000080419326,0.000013274448,0.000012864429,0.000029610756,0.000030045836,0.0010495071],"genre_scores_gemma":[0.99839264,0.000031050782,0.001288187,0.000013580421,0.0000049847927,0.000009864516,0.000028873066,0.000008878806,0.00022191429],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999175,0.000027363865,0.0000041691956,0.0000108707545,0.000012406365,0.000027690436],"domain_scores_gemma":[0.99971634,0.00009157216,0.0000680051,0.00002417189,0.000041745334,0.000058189933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030061093,0.00038562185,0.000450512,0.0003705918,0.0005876864,0.00050342316,0.00058420456,0.0006735897,0.0010575015],"category_scores_gemma":[0.0009769491,0.00030937692,0.000568037,0.00023830529,0.00055993744,0.00043539,0.00046099856,0.00039260258,0.000074389834],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006744368,0.00006891287,0.008089815,0.000029398674,0.00005272438,0.00041207153,0.00010437377,0.9830609,0.0038012601,0.0034304175,0.0001018207,0.0007808975],"study_design_scores_gemma":[0.000022645047,0.000034015284,0.0012552532,0.0000018713849,0.000007406287,0.000019409239,0.000029184297,0.9978562,0.00032846024,0.0003809261,0.000060186478,0.0000044760395],"about_ca_topic_score_codex":0.008839618,"about_ca_topic_score_gemma":0.0031209267,"teacher_disagreement_score":0.008839618,"about_ca_system_score_codex":0.000602732,"about_ca_system_score_gemma":0.00046788456,"threshold_uncertainty_score":0.017576337},"labels":[],"label_agreement":null},{"id":"W2020844421","doi":"10.1088/0004-637x/703/1/l81","title":"DENSE IRON EJECTA AND CORE-COLLAPSE SUPERNOVA EXPLOSION IN THE YOUNG SUPERNOVA REMNANT G11.2-0.3","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Ejecta; Physics; Supernova remnant; Astrophysics; Supernova; Type II supernova; Pulsar wind nebula; Protein filament; Astronomy; Cassiopeia A","score_opus":0.016275884950671473,"score_gpt":0.2418023619186867,"score_spread":0.22552647696801523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020844421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998068,0.00003300542,0.000022197666,0.0000027026124,5.2634624e-7,0.0000018317792,0.00003767454,0.000003057757,0.00009227118],"genre_scores_gemma":[0.99928916,0.000039602004,0.00008309004,0.000012378342,0.0000024614396,0.0000024899912,0.00042789607,0.0000025443012,0.00014025973],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999589,0.0000038142234,0.0000024156745,0.000011891954,0.000008075689,0.000014917104],"domain_scores_gemma":[0.99982685,0.000016805176,0.000063944426,0.000012432944,0.0000116313495,0.00006836626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012702511,0.0003226665,0.00020013613,0.00048912456,0.00020325866,0.00025457912,0.00014785609,0.00022962535,0.00040111132],"category_scores_gemma":[0.0001558823,0.00013686097,0.00020593553,0.00025186833,0.00021437448,0.00009899023,0.00031354948,0.00021111924,0.000113153634],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010656654,0.00019329049,0.8725017,0.000023325836,0.0000888806,0.0025760627,0.00020647216,0.0002572471,0.11929393,0.000083444655,0.00013307789,0.0035770033],"study_design_scores_gemma":[0.000006285435,0.00008408976,0.99810153,9.834276e-7,0.000008345492,0.00070404843,0.000032772157,0.00011283736,0.00084650825,0.000012207361,0.000088036606,0.0000024340372],"about_ca_topic_score_codex":0.0052651013,"about_ca_topic_score_gemma":0.0077150073,"teacher_disagreement_score":0.0052651013,"about_ca_system_score_codex":0.00023322366,"about_ca_system_score_gemma":0.00008773929,"threshold_uncertainty_score":0.0104689},"labels":[],"label_agreement":null},{"id":"W2020861493","doi":"10.1086/527436","title":"On the White Dwarf Cooling Sequence of the Globular Cluster ω Centauri","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Hubble space telescope; White dwarf; Horizontal branch; Photometry (optics); Star cluster; Astronomy; Advanced Camera for Surveys; Stars; Hertzsprung–Russell diagram; Stellar evolution","score_opus":0.018353115520528557,"score_gpt":0.22457407018826514,"score_spread":0.20622095466773657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020861493","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987534,0.00010658586,0.00014348044,0.000007829564,0.0000028413244,0.0000016981021,0.00018124243,0.000009130401,0.0007937375],"genre_scores_gemma":[0.9988673,0.000048733615,0.00016800842,0.000007337844,0.0000055868168,0.0000026481669,0.00058210583,0.0000040580544,0.00031421141],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999926,0.000009486715,0.0000027340789,0.000027953585,0.000011411155,0.000022383907],"domain_scores_gemma":[0.9995863,0.00010508291,0.000121952144,0.00004189252,0.00005441532,0.00009034436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015389045,0.00018867094,0.00010867668,0.0010095629,0.0003306734,0.00022780903,0.00016847676,0.0001287962,0.0013781132],"category_scores_gemma":[0.00074767735,0.00008051314,0.000092059796,0.00045938342,0.0002482625,0.00019153993,0.00026894707,0.00009536761,0.00032189194],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032262816,0.0000215845,0.9591837,0.000039872,0.00003066849,0.00036708123,0.00031625733,0.0007657345,0.018731562,0.00059326587,0.0005422598,0.019085424],"study_design_scores_gemma":[0.0000012716667,0.000015618552,0.9985952,0.000003206044,0.000005072023,0.000099611534,0.000022317989,0.00040145515,0.0003600636,0.000089325185,0.0004050787,0.000001827878],"about_ca_topic_score_codex":0.0044407966,"about_ca_topic_score_gemma":0.007985513,"teacher_disagreement_score":0.0044407966,"about_ca_system_score_codex":0.00022763034,"about_ca_system_score_gemma":0.00009983021,"threshold_uncertainty_score":0.008829892},"labels":[],"label_agreement":null},{"id":"W2020888000","doi":"10.1088/0004-637x/728/2/95","title":"EVIDENCE FOR A MASSIVE NEUTRON STAR FROM A RADIAL-VELOCITY STUDY OF THE COMPANION TO THE BLACK-WIDOW PULSAR PSR B1957+20","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":285,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Pulsar; Neutron star; Astrophysics; Amplitude; Millisecond pulsar; Radial velocity; Proper motion; Astronomy; X-ray pulsar; Mass ratio; Star (game theory); Stars","score_opus":0.0629200328058365,"score_gpt":0.33900787926164155,"score_spread":0.2760878464558051,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020888000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99858785,0.00014219157,0.0002397894,0.000021868842,0.0000071717445,0.0000032877756,0.00004900802,0.000015191954,0.0009337921],"genre_scores_gemma":[0.9993309,0.000059207876,0.0002839212,0.000027376544,0.000009579882,0.0000019176473,0.0001218753,0.000005262721,0.0001600924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994206,0.0000049314285,0.0000051435472,0.000017540648,0.000017745246,0.00001252534],"domain_scores_gemma":[0.99966455,0.000036744535,0.00014626054,0.000027197713,0.000028484943,0.0000968276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021554809,0.00025272398,0.00017145363,0.0008140943,0.00042903543,0.00040197908,0.0002166281,0.00032785267,0.0011759043],"category_scores_gemma":[0.00045117535,0.00016488046,0.0001672684,0.0004152083,0.00026871564,0.00023606376,0.0004871143,0.0002240149,0.00025595372],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048382673,0.0000858203,0.62817854,0.000072380295,0.000102166174,0.0015368467,0.00048799635,0.00023253246,0.35409096,0.0009728206,0.0003331553,0.013422887],"study_design_scores_gemma":[0.000023005708,0.0002816135,0.9771756,0.000013335321,0.000060851748,0.001815734,0.00019778115,0.0010820287,0.016916087,0.00034968642,0.0020731646,0.000011125703],"about_ca_topic_score_codex":0.0008357227,"about_ca_topic_score_gemma":0.001993199,"teacher_disagreement_score":0.0011759043,"about_ca_system_score_codex":0.00015211801,"about_ca_system_score_gemma":0.00009926474,"threshold_uncertainty_score":0.0039337873},"labels":[],"label_agreement":null},{"id":"W2020889659","doi":"10.1086/498707","title":"Colors of Luminous Bulges in Cluster MS 1054-03 and Field Galaxies at Redshifts <i>z</i>  ~ 0.83","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Hubble space telescope; Elliptical galaxy; Galaxy; Luminosity; Astronomy; Redshift; Advanced Camera for Surveys","score_opus":0.005231720948618224,"score_gpt":0.20266706618190974,"score_spread":0.1974353452332915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020889659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99961424,0.000019622355,0.000017497914,0.0000049015616,4.868845e-7,6.832213e-7,0.000120416385,0.000008214633,0.00021402663],"genre_scores_gemma":[0.99947983,0.000013640677,0.000045112196,0.0000072087887,0.0000014823013,0.0000014836165,0.00033254913,0.0000023278856,0.000116399555],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991095,0.000010177625,0.000007531181,0.000026399655,0.000015225523,0.000029738656],"domain_scores_gemma":[0.99940085,0.000092319504,0.00020805336,0.000044272154,0.000045264722,0.00020928538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001781792,0.00016959742,0.00020868443,0.0021103744,0.000435374,0.0004918116,0.00023402467,0.00021875353,0.0014093254],"category_scores_gemma":[0.00046982907,0.00017062986,0.0001873026,0.0009499784,0.00044601256,0.00020984067,0.00046190407,0.00021388265,0.00021354969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026063222,0.000045897483,0.9865089,0.000013851548,0.00004466514,0.000070710936,0.00058037625,0.00040952087,0.0082079405,0.00014914827,0.0003234064,0.0033849624],"study_design_scores_gemma":[0.0000018550164,0.000011651392,0.9995363,8.747315e-7,0.000004927613,0.00003122722,0.00009716556,0.00011466941,0.00015264074,0.000012836395,0.00003457082,0.0000014227272],"about_ca_topic_score_codex":0.021525329,"about_ca_topic_score_gemma":0.025416227,"teacher_disagreement_score":0.021525329,"about_ca_system_score_codex":0.000691305,"about_ca_system_score_gemma":0.00011371611,"threshold_uncertainty_score":0.04280007},"labels":[],"label_agreement":null},{"id":"W2020940073","doi":"10.1088/0004-637x/703/1/939","title":"THE GLOBULAR CLUSTER SYSTEM IN M87: A WIDE-FIELD STUDY WITH CFHT/MEGACAM","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Metallicity; Horizontal branch; Cluster (spacecraft); Luminosity; Red-giant branch; Population; Stellar population","score_opus":0.004252585457848925,"score_gpt":0.20327487275186157,"score_spread":0.19902228729401264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2020940073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987974,0.00012171003,0.000043312204,0.000022952494,0.0000012246297,0.000007590847,0.0005773185,0.0000051637967,0.00042337112],"genre_scores_gemma":[0.99729437,0.00012905516,0.0002192237,0.00004734796,0.000013932652,0.000008196193,0.0020164666,0.000006406817,0.0002650066],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999706,0.00003959945,0.000013583198,0.00005938111,0.000067401284,0.00011400667],"domain_scores_gemma":[0.999469,0.00005969341,0.00010266873,0.00007173464,0.00008571719,0.00021123835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005604428,0.00030808977,0.00037942125,0.0024521635,0.0007081949,0.00044366505,0.0005121234,0.00046411305,0.00093473995],"category_scores_gemma":[0.00047388097,0.00022123175,0.00028910133,0.0025275925,0.00041341953,0.00040609064,0.0009934163,0.00029011743,0.00058958796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016915408,0.00016637381,0.9834141,0.00003108991,0.00007541073,0.0008677244,0.0011102515,0.00022070565,0.0030209783,0.0001447561,0.0013993622,0.009379994],"study_design_scores_gemma":[0.0000027426408,0.00001918076,0.9993488,0.0000029870853,0.000005624776,0.00011167417,0.00014568266,0.00009958722,0.00005052373,0.0000065642935,0.00020493982,0.0000017006546],"about_ca_topic_score_codex":0.04690387,"about_ca_topic_score_gemma":0.079569474,"teacher_disagreement_score":0.04690387,"about_ca_system_score_codex":0.0006092109,"about_ca_system_score_gemma":0.0003263172,"threshold_uncertainty_score":0.09326172},"labels":[],"label_agreement":null},{"id":"W2021008553","doi":"10.1086/309323","title":"The Origin of Star Formation Gradients in Rich Galaxy Clusters","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":740,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Astrophysics; Physics; Galaxy cluster; Astronomy; Virial theorem; Cluster (spacecraft); Accretion (finance); Elliptical galaxy; Galaxy; Star formation; Virial mass; Star cluster; Context (archaeology); Geography","score_opus":0.007349622583377528,"score_gpt":0.21452015114176945,"score_spread":0.2071705285583919,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021008553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99813193,0.00007423217,0.0005115571,0.000053515534,0.0000016249384,0.000003308873,0.000026512507,0.00003644295,0.0011608793],"genre_scores_gemma":[0.9996749,0.000022534623,0.00012474919,0.000007887813,0.000001649394,0.000001128328,0.000015513779,0.000005463895,0.00014607556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993086,0.000012640977,0.0000020841971,0.000016792921,0.000012545211,0.000025179967],"domain_scores_gemma":[0.9992212,0.00018151608,0.00024799048,0.000075711556,0.00008043819,0.00019316336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022558749,0.0001619746,0.00021684406,0.00046804984,0.00036833234,0.00067606545,0.00038152008,0.00028836523,0.00081721606],"category_scores_gemma":[0.0017776366,0.00019871136,0.00023723097,0.00028033095,0.0005334459,0.00032289056,0.0005827192,0.0002578719,0.000108612345],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006120388,0.00007102948,0.768365,0.00009806715,0.00016436505,0.0008502724,0.0020879623,0.13219674,0.039537482,0.04232517,0.001171826,0.012520112],"study_design_scores_gemma":[0.00008320362,0.00009802071,0.8023194,0.000024397727,0.00007193534,0.00033943998,0.00052480964,0.17020477,0.0054832627,0.018248582,0.0025339688,0.000068232555],"about_ca_topic_score_codex":0.016151115,"about_ca_topic_score_gemma":0.009653763,"teacher_disagreement_score":0.016151115,"about_ca_system_score_codex":0.0011174547,"about_ca_system_score_gemma":0.00032891365,"threshold_uncertainty_score":0.032114267},"labels":[],"label_agreement":null},{"id":"W2021113739","doi":"10.1088/0004-637x/779/1/90","title":"ERRATUM: “COSMOLOGICAL SIMULATIONS OF INTERGALACTIC MEDIUM EVOLUTION. I. TEST OF THE SUBGRID CHEMICAL ENRICHMENT MODEL” (2013, ApJ, 777, 107)","year":2013,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Scientific Research and Discoveries","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"Eusko Jaurlaritza","keywords":"Physics; Intergalactic medium; Astrophysics; Statistical physics; Redshift; Galaxy","score_opus":0.015139434490026674,"score_gpt":0.2585611571186406,"score_spread":0.24342172262861392,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021113739","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.002592567,0.0014420596,0.0021178455,0.065447584,0.88838327,0.000069760645,0.01670256,0.0018233472,0.02142096],"genre_scores_gemma":[0.07037712,0.008266473,0.013770626,0.07655721,0.10351033,0.00036777722,0.05456631,0.008522773,0.6640614],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.998522,0.00015650723,0.00019092059,0.00016531862,0.0008518956,0.000113319045],"domain_scores_gemma":[0.99105823,0.002479789,0.00049445865,0.0006394533,0.0048289536,0.0004990763],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015911238,0.001509361,0.0013020148,0.001990167,0.0034634285,0.0032682088,0.0027306785,0.0028799318,0.07467638],"category_scores_gemma":[0.021241685,0.0008924532,0.0013618362,0.002285482,0.0013360981,0.002476465,0.0019856195,0.004169878,0.030887209],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005776331,0.00001123882,0.00013154073,0.00004458906,0.000010578667,0.000113639115,0.000012985019,0.00030545428,0.00008049786,0.00083493296,0.99573815,0.0026587285],"study_design_scores_gemma":[0.000330933,0.00007542502,0.0051431055,0.00032201613,0.00012981553,0.0004874905,0.00022802985,0.004300862,0.0024990141,0.007473867,0.97881764,0.00019179125],"about_ca_topic_score_codex":0.036277503,"about_ca_topic_score_gemma":0.04717495,"teacher_disagreement_score":0.07467638,"about_ca_system_score_codex":0.0032851964,"about_ca_system_score_gemma":0.0038591232,"threshold_uncertainty_score":0.24981737},"labels":[],"label_agreement":null},{"id":"W2021171692","doi":"10.1086/500962","title":"Variations in D/H and D/O from New<i>Far Ultraviolet Spectroscopic Explorer</i>Observations","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Ultraviolet; Far ultraviolet; Ultraviolet astronomy; Range (aeronautics); Vacuum ultraviolet; Interstellar medium; Ionization; Hubble space telescope; Spectral line","score_opus":0.01461869240826359,"score_gpt":0.2284387174076349,"score_spread":0.21382002499937133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021171692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99236745,0.00014283494,0.0006238779,0.000039441125,0.000013436648,0.0000099477165,0.0035088554,0.00011275975,0.003181254],"genre_scores_gemma":[0.98891056,0.0001327882,0.001262871,0.000050251216,0.00001786524,0.000019230378,0.0088251615,0.000039578583,0.00074151374],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984777,0.000007252949,0.000010500976,0.00005084926,0.00005306404,0.000030628686],"domain_scores_gemma":[0.9995117,0.000040097704,0.00021090839,0.000035155786,0.000059975177,0.00014215695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002147931,0.00028970835,0.00016828426,0.0012206412,0.00022420315,0.0004761007,0.00028025426,0.00019012233,0.0011136789],"category_scores_gemma":[0.00041344872,0.00016700863,0.00024040414,0.00082577876,0.00015230523,0.0002918218,0.0005501563,0.0002738313,0.00036921247],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018046037,0.00010064239,0.9376915,0.000065022134,0.00013122636,0.0002757111,0.00026914504,0.0010463417,0.04310546,0.0001939526,0.002144904,0.014795603],"study_design_scores_gemma":[0.000012863367,0.000024011018,0.99372226,0.0000073740566,0.000019716259,0.00010271962,0.00006526249,0.0008921116,0.002675587,0.00006392005,0.00240467,0.000009550531],"about_ca_topic_score_codex":0.006741467,"about_ca_topic_score_gemma":0.02200905,"teacher_disagreement_score":0.006741467,"about_ca_system_score_codex":0.00047107245,"about_ca_system_score_gemma":0.00012519155,"threshold_uncertainty_score":0.013404429},"labels":[],"label_agreement":null},{"id":"W2021216634","doi":"10.1086/509819","title":"Nonradial Oscillations on a Pre–Main‐Sequence Star","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Oscillation (cell signaling); Star (game theory); Astrophysics; Spectral line; Sequence (biology); Position (finance); Diagram; Main sequence; Asteroseismology; Stars; Astronomy","score_opus":0.017621841809081565,"score_gpt":0.2566767337397553,"score_spread":0.23905489193067375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021216634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976935,0.000049636637,0.0011430152,0.000011753945,0.0000017402716,0.000002015905,0.00007689706,0.000033979784,0.0009873537],"genre_scores_gemma":[0.99906987,0.000033104494,0.0005883899,0.000003131947,0.0000025359,0.0000017469206,0.00010610313,0.000003933643,0.00019123095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999682,0.0000063855014,0.0000012765157,0.000010488057,0.0000077246,0.0000059364543],"domain_scores_gemma":[0.9998154,0.000052451232,0.00004219775,0.000042584394,0.000022060427,0.000025344849],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011791459,0.00019113345,0.00014972728,0.00016669935,0.00018978542,0.00016746868,0.00019086993,0.00011730573,0.0008825379],"category_scores_gemma":[0.00040333098,0.00008421451,0.0001819607,0.00016447627,0.00016742319,0.00016268506,0.00021754277,0.000120106466,0.0002046571],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006502505,0.000119086006,0.5859292,0.00014578093,0.0001557813,0.0012484017,0.00052866404,0.2185129,0.1353999,0.0058135055,0.0009925675,0.050503977],"study_design_scores_gemma":[0.00004726717,0.0003576701,0.67196095,0.000020548563,0.00006232332,0.00061169226,0.00011419771,0.30660996,0.012401178,0.0056602536,0.0021328474,0.000021057174],"about_ca_topic_score_codex":0.0037672725,"about_ca_topic_score_gemma":0.00655435,"teacher_disagreement_score":0.0037672725,"about_ca_system_score_codex":0.00021312496,"about_ca_system_score_gemma":0.00013861935,"threshold_uncertainty_score":0.0074906945},"labels":[],"label_agreement":null},{"id":"W2021222547","doi":"10.1086/589962","title":"Particle Acceleration by Fast Modes in Solar Flares","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Solar flare; Acceleration; Particle acceleration; Cascade; Electron; Scattering; Flare; Solar energetic particles; Plasma","score_opus":0.01068485407355366,"score_gpt":0.22130816362146072,"score_spread":0.21062330954790706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021222547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9296092,0.0008836681,0.06268744,0.00023580341,0.000050036473,0.00002955868,0.000041346386,0.00013658791,0.0063263616],"genre_scores_gemma":[0.9954573,0.00031986713,0.0027926925,0.000017845654,0.000027671753,0.000010739931,0.000024330782,0.000014853591,0.0013346775],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999651,0.000009265753,0.0000012029654,0.0000049401656,0.000009987511,0.000009508851],"domain_scores_gemma":[0.99978477,0.00008352892,0.00006343379,0.000015628839,0.000028728347,0.000023956645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017570486,0.00049375393,0.0002005258,0.00035997762,0.00032091633,0.00038606155,0.00029690922,0.0004053108,0.0011688443],"category_scores_gemma":[0.0007648563,0.00015188451,0.00027272062,0.0001805308,0.0002526464,0.00043275522,0.00047416176,0.00034464072,0.00015018859],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003710017,0.00014481478,0.020805927,0.00020519203,0.00011528509,0.001375535,0.00050107326,0.7424438,0.06508421,0.13170917,0.0013864741,0.035857502],"study_design_scores_gemma":[0.000037012367,0.000110297435,0.0036609957,0.0000056572458,0.000010385618,0.0001540508,0.000040039227,0.969464,0.0020537057,0.02390399,0.00054853666,0.0000113302185],"about_ca_topic_score_codex":0.0015119546,"about_ca_topic_score_gemma":0.0007296796,"teacher_disagreement_score":0.0015119546,"about_ca_system_score_codex":0.0002145698,"about_ca_system_score_gemma":0.0001296825,"threshold_uncertainty_score":0.003910184},"labels":[],"label_agreement":null},{"id":"W2021296731","doi":"10.1088/0004-637x/772/1/77","title":"HerMES: COSMIC INFRARED BACKGROUND ANISOTROPIES AND THE CLUSTERING OF DUSTY STAR-FORMING GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":171,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Halo; Luminosity; Astronomy; Dark matter halo; Cosmic infrared background; Luminous infrared galaxy; Star formation; Dark matter; Anisotropy; Cosmic microwave background","score_opus":0.00911031584823331,"score_gpt":0.2079636429884962,"score_spread":0.19885332714026288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021296731","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.951719,0.002646404,0.0051569613,0.0014690737,0.0001384888,0.000022543365,0.009677569,0.0007493062,0.02842057],"genre_scores_gemma":[0.99304104,0.00041737987,0.0007174798,0.000061867344,0.000108547756,0.0000061957594,0.0027315174,0.00009114167,0.0028247503],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999796,0.00005332305,0.0000078923495,0.000062897765,0.000049265225,0.00003069365],"domain_scores_gemma":[0.99843055,0.0002699505,0.00068979955,0.00022384187,0.000104237806,0.0002815237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004312807,0.00023592763,0.00026708707,0.000749475,0.00026805367,0.00090770447,0.00025806372,0.00018966278,0.008010069],"category_scores_gemma":[0.0022627283,0.0001156848,0.0001694791,0.001330154,0.00026335331,0.00043019155,0.0005421095,0.00035540306,0.0011360743],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016855441,0.000052893884,0.931967,0.000049720256,0.00025355406,0.00009366876,0.00024414746,0.0029893399,0.0012630519,0.007860625,0.015452915,0.039604522],"study_design_scores_gemma":[0.000008023601,0.000014137161,0.98674357,0.000015712354,0.00002882342,0.00009816861,0.0001233548,0.0018958187,0.00010278126,0.0050563533,0.005902758,0.000010520404],"about_ca_topic_score_codex":0.011730396,"about_ca_topic_score_gemma":0.012283447,"teacher_disagreement_score":0.011730396,"about_ca_system_score_codex":0.0003340874,"about_ca_system_score_gemma":0.00018179748,"threshold_uncertainty_score":0.026796341},"labels":[],"label_agreement":null},{"id":"W2021397202","doi":"10.1086/432678","title":"Radiative Transfer and Acceleration in Magnetocentrifugal Winds","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":181,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Radiative transfer; Physics; Acceleration; Outflow; Atmospheric radiative transfer codes; Astrophysics; Computational physics; Atmospheric sciences; Mechanics; Meteorology; Classical mechanics; Optics","score_opus":0.008618590747080105,"score_gpt":0.22835819070652166,"score_spread":0.21973959995944156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021397202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97490054,0.00032163135,0.01300334,0.0001664563,0.000027058428,0.00002115877,0.000057152603,0.00009354242,0.011409013],"genre_scores_gemma":[0.997928,0.00009290779,0.0004992962,0.000019499155,0.000009608768,0.0000067044584,0.000025927327,0.000009874625,0.0014080992],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99992645,0.000017757091,0.0000023280375,0.000011419685,0.00001317623,0.0000287136],"domain_scores_gemma":[0.9998977,0.000024739335,0.000025426492,0.0000136381195,0.000011679862,0.000026878479],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016519471,0.00050457515,0.00029329816,0.00023499998,0.0003490587,0.00062599726,0.0005075263,0.0007182584,0.001503122],"category_scores_gemma":[0.0005937435,0.0002961612,0.0005870255,0.00014445024,0.00038701782,0.0006272918,0.00080237107,0.00028707733,0.00020114853],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030057775,0.00012940842,0.036229085,0.00009993769,0.000100761376,0.0016384418,0.00034333864,0.80060875,0.059012987,0.087969355,0.000884573,0.012682814],"study_design_scores_gemma":[0.0001198115,0.00012680772,0.01894526,0.000010542773,0.000025666566,0.00035320068,0.00009998433,0.95909387,0.0038223988,0.016292874,0.0010726767,0.00003690312],"about_ca_topic_score_codex":0.0027173285,"about_ca_topic_score_gemma":0.0014578084,"teacher_disagreement_score":0.0027173285,"about_ca_system_score_codex":0.0006227063,"about_ca_system_score_gemma":0.00020973665,"threshold_uncertainty_score":0.0054029822},"labels":[],"label_agreement":null},{"id":"W2021427471","doi":"10.1086/429690","title":"<i>FUSE</i>Measurements of Far‐Ultraviolet Extinction. I. Galactic Sight Lines","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Extinction (optical mineralogy); Ultraviolet; Astrophysics; Physics; Extrapolation; Line-of-sight; Astronomy; Infrared; Optics","score_opus":0.020039895347039788,"score_gpt":0.25177004010360626,"score_spread":0.23173014475656648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021427471","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91230124,0.0016347894,0.0035603202,0.00014125684,0.000045640267,0.000023656348,0.048348263,0.0013037655,0.032641128],"genre_scores_gemma":[0.9673813,0.0004841147,0.0034271856,0.00008919432,0.000025281122,0.000012461635,0.0271342,0.000060526196,0.0013857551],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991727,0.0000052071864,0.0000077701025,0.000018701827,0.000032369593,0.000018617142],"domain_scores_gemma":[0.99964166,0.000047154514,0.00015130323,0.000041086674,0.000071821116,0.00004684564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012436094,0.00026607953,0.000116717274,0.0022200085,0.00028902388,0.0003352974,0.00021634201,0.00027642527,0.0019901518],"category_scores_gemma":[0.000450886,0.000065384345,0.00020670235,0.0010775502,0.000116744326,0.0003553158,0.00024224623,0.00022810746,0.0005845223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037413128,0.000118717544,0.8518934,0.00020780809,0.00027392083,0.00039073534,0.00038780237,0.0046570604,0.06426126,0.0016381358,0.020991256,0.054805793],"study_design_scores_gemma":[0.000005511995,0.00006563782,0.97317106,0.000016702807,0.00004327291,0.00041057254,0.0000621767,0.0012525022,0.011616553,0.00030272477,0.013036283,0.000016994567],"about_ca_topic_score_codex":0.01186017,"about_ca_topic_score_gemma":0.013873372,"teacher_disagreement_score":0.01186017,"about_ca_system_score_codex":0.0003532188,"about_ca_system_score_gemma":0.00008586012,"threshold_uncertainty_score":0.02358228},"labels":[],"label_agreement":null},{"id":"W2021458521","doi":"10.1088/0004-637x/732/2/88","title":"NEUTRON STAR RADIUS MEASUREMENT WITH THE QUIESCENT LOW-MASS X-RAY BINARY U24 IN NGC 6397","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"RADIUS; Globular cluster; Neutron star; Flux (metallurgy); Atmosphere (unit); Binary number; Spectral line; Pulsar; Range (aeronautics)","score_opus":0.02446793248183369,"score_gpt":0.20477053911736529,"score_spread":0.1803026066355316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021458521","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99960333,0.000043910637,0.00007206919,0.0000022295983,8.893901e-7,0.0000013747347,0.000057157104,0.00001004119,0.0002090754],"genre_scores_gemma":[0.99937385,0.000029526445,0.00027312667,0.0000021121903,0.0000024526362,0.0000035789626,0.00019311457,0.0000046540813,0.00011743224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998336,0.00001566812,0.000016369235,0.000049035476,0.000053104093,0.00003218347],"domain_scores_gemma":[0.9996014,0.000039337974,0.0001753811,0.00005075036,0.00005665236,0.000076447766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022557846,0.00016764076,0.0003886957,0.001133406,0.00049507775,0.0006082315,0.00040786364,0.00027959052,0.0006536878],"category_scores_gemma":[0.00084924564,0.00012833145,0.00019539242,0.0008776435,0.00024134805,0.00019640106,0.0005295565,0.00016402741,0.00028136343],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054092816,0.00005549668,0.9117524,0.00003907682,0.0000768691,0.0007662019,0.0008209653,0.00085324066,0.07325772,0.00011251434,0.00019597828,0.011528663],"study_design_scores_gemma":[0.000010519154,0.000093298186,0.991015,0.000006645264,0.000028702487,0.0004436573,0.00020840752,0.0009943808,0.006608719,0.000028346893,0.00055325415,0.000009085815],"about_ca_topic_score_codex":0.006508699,"about_ca_topic_score_gemma":0.011897346,"teacher_disagreement_score":0.006508699,"about_ca_system_score_codex":0.0003843897,"about_ca_system_score_gemma":0.00012762207,"threshold_uncertainty_score":0.0129416585},"labels":[],"label_agreement":null},{"id":"W2021547380","doi":"10.1088/0004-637x/723/2/1294","title":"EMBEDDED PROTOSTELLAR DISKS AROUND (SUB-)SOLAR PROTOSTARS. I. DISK STRUCTURE AND EVOLUTION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Gravitational collapse; Protostar; Brown dwarf; Gravitation; Gravitational energy; Star formation; Amplitude; Molecular cloud; Stellar evolution","score_opus":0.005281178891480357,"score_gpt":0.22590229012170862,"score_spread":0.22062111123022826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021547380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980248,0.00011969307,0.0005797334,0.000020556372,0.0000049617547,0.00001008068,0.00021694275,0.000031578365,0.0009916397],"genre_scores_gemma":[0.997412,0.00012868836,0.0016347494,0.000014178452,0.0000061596816,0.000009913856,0.00038779,0.000014267447,0.00039225566],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995136,0.000008100172,0.0000030914814,0.000012509006,0.000008643838,0.000016257383],"domain_scores_gemma":[0.99980384,0.000054430955,0.000052446223,0.000022295575,0.000022831004,0.000044165663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008092596,0.00029556063,0.0002654337,0.0003418421,0.00038142223,0.00052685256,0.00063740043,0.00044450766,0.0009132849],"category_scores_gemma":[0.00049764,0.00021252109,0.00037805666,0.00042024397,0.00039616087,0.00030761663,0.00040149043,0.00025268036,0.00018258776],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032130053,0.0004405738,0.15845783,0.00013019504,0.00017020408,0.0010649671,0.00040153725,0.79183364,0.03457347,0.0029958729,0.000602431,0.009007909],"study_design_scores_gemma":[0.000073147115,0.00017859938,0.07258981,0.000011359121,0.000041573563,0.00034997187,0.00024029761,0.9208278,0.00349946,0.0010156188,0.001150414,0.00002202],"about_ca_topic_score_codex":0.010674817,"about_ca_topic_score_gemma":0.0050514643,"teacher_disagreement_score":0.010674817,"about_ca_system_score_codex":0.0006578339,"about_ca_system_score_gemma":0.00027796364,"threshold_uncertainty_score":0.021225333},"labels":[],"label_agreement":null},{"id":"W2021555682","doi":"10.1088/0004-637x/776/1/1","title":"THREE-DIMENSIONAL HYDRODYNAMIC SIMULATIONS OF MULTIPHASE GALACTIC DISKS WITH STAR FORMATION FEEDBACK. I. REGULATION OF STAR FORMATION RATES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":202,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Star formation; Turbulence; Interstellar medium; Stars; Angular momentum; Scaling; Momentum (technical analysis); Star (game theory); Thermal","score_opus":0.01037659554510113,"score_gpt":0.2368555034587913,"score_spread":0.2264789079136902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021555682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97614187,0.00031651914,0.005943304,0.0009985553,0.000116325005,0.00012320503,0.0018834035,0.00028239025,0.014194314],"genre_scores_gemma":[0.99028873,0.00016716578,0.0056361347,0.00026542318,0.000035451132,0.00016380874,0.0013142353,0.00008110668,0.0020479783],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996762,0.000080573955,0.000024553921,0.000047720652,0.00006875143,0.00010213157],"domain_scores_gemma":[0.9978551,0.0010210742,0.0002354758,0.00009952974,0.00032662286,0.00046201723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045413643,0.00085104845,0.0010508192,0.00084121997,0.0013281747,0.0014065673,0.0018342913,0.0023395715,0.003830487],"category_scores_gemma":[0.0029773433,0.00067744596,0.0010497005,0.0009420099,0.0017482917,0.0008597443,0.0012724997,0.0018730537,0.0003264912],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018276004,0.00022631841,0.006378955,0.000040072384,0.000068306836,0.00016314231,0.00010094421,0.9885123,0.00079743436,0.0021098957,0.000566929,0.0008529279],"study_design_scores_gemma":[0.000064335814,0.00003475463,0.0012677767,0.0000075834564,0.000009011763,0.0000108096,0.000056511028,0.99757665,0.00017198693,0.00052634475,0.00026324182,0.00001093729],"about_ca_topic_score_codex":0.061446678,"about_ca_topic_score_gemma":0.030452859,"teacher_disagreement_score":0.061446678,"about_ca_system_score_codex":0.0028866632,"about_ca_system_score_gemma":0.0016375475,"threshold_uncertainty_score":0.12217802},"labels":[],"label_agreement":null},{"id":"W2021570256","doi":"10.1088/0004-637x/786/2/78","title":"WIDE-FIELD<i>HUBBLE SPACE TELESCOPE</i>OBSERVATIONS OF THE GLOBULAR CLUSTER SYSTEM IN NGC 1399","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Space (punctuation); Cluster (spacecraft); Hubble space telescope; Elliptical galaxy","score_opus":0.0067247829246235855,"score_gpt":0.19479459537482377,"score_spread":0.18806981245020019,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021570256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99461454,0.000082929124,0.000082630395,0.000062448285,0.000006011033,0.000003842097,0.0010847901,0.0000128311585,0.0040498553],"genre_scores_gemma":[0.996651,0.000063112784,0.00025425453,0.000024085943,0.0000075444423,0.000003683392,0.0017940768,0.000006141496,0.0011961025],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991596,0.0000061129535,0.000004319251,0.000028709439,0.000024801915,0.000020163852],"domain_scores_gemma":[0.99969614,0.000019837775,0.000090905196,0.00002709561,0.000060482387,0.0001054571],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017475484,0.00007079943,0.00009934883,0.0011993679,0.0006078939,0.00036270433,0.00023180396,0.00019957588,0.0021106023],"category_scores_gemma":[0.0003081629,0.00008289642,0.0000851053,0.0011908874,0.000289533,0.00027518885,0.00051519397,0.00019081372,0.00039849695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009640638,0.000073771414,0.9523426,0.000025350197,0.000035721525,0.00021910299,0.00051226,0.0003254544,0.029490521,0.00078824215,0.0030576834,0.013032934],"study_design_scores_gemma":[0.0000022648592,0.000004880516,0.99804723,0.0000033858519,0.000003478666,0.000037619284,0.00014106702,0.00008753021,0.00019530322,0.000065044944,0.0014103674,0.0000017230748],"about_ca_topic_score_codex":0.080861494,"about_ca_topic_score_gemma":0.19097875,"teacher_disagreement_score":0.080861494,"about_ca_system_score_codex":0.0007428115,"about_ca_system_score_gemma":0.0004763058,"threshold_uncertainty_score":0.16078168},"labels":[],"label_agreement":null},{"id":"W2021601212","doi":"10.1086/383518","title":"Photoevaporation of Circumstellar Disks around Young Stars","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":252,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Astrophysics; T Tauri star; Stars; Forbidden mechanism; Line (geometry); Spectral line; Photoevaporation; Emission spectrum; Radial velocity; Astronomy; Protoplanetary disk","score_opus":0.011706976803502113,"score_gpt":0.23868001497279676,"score_spread":0.22697303816929465,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021601212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972357,0.00007941531,0.0013365437,0.000054069424,0.0000051635857,0.000008609699,0.00003930379,0.00004119069,0.0012000507],"genre_scores_gemma":[0.99913955,0.00008401521,0.00045187832,0.000011428373,0.000006476149,0.0000052212495,0.00003509892,0.000008339603,0.00025797097],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99995613,0.000009610188,0.0000017876208,0.00000804235,0.0000074808536,0.000016895418],"domain_scores_gemma":[0.99961144,0.00013982248,0.00012201885,0.000020722473,0.000022586937,0.000083333834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011667878,0.00035071382,0.0002904642,0.0002775161,0.0005893307,0.00049346057,0.0005577812,0.00038917531,0.00073491107],"category_scores_gemma":[0.00077635807,0.0001857172,0.00025799018,0.00027157142,0.0007679614,0.00047768737,0.00065817154,0.00034556768,0.00016443942],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003143918,0.0002420251,0.057976663,0.00008903342,0.000084919426,0.001793648,0.0005254979,0.8987005,0.028287696,0.0055550346,0.00063969404,0.0057908334],"study_design_scores_gemma":[0.00012963967,0.00023206312,0.014335933,0.000006781681,0.000021643194,0.00016776267,0.00019217932,0.9762526,0.0048236023,0.0033238195,0.00049523707,0.000018736555],"about_ca_topic_score_codex":0.0055033052,"about_ca_topic_score_gemma":0.0022775407,"teacher_disagreement_score":0.0055033052,"about_ca_system_score_codex":0.0007957951,"about_ca_system_score_gemma":0.00031468656,"threshold_uncertainty_score":0.010942519},"labels":[],"label_agreement":null},{"id":"W2021631795","doi":"10.1088/0004-637x/746/1/88","title":"OPTICAL AND INFRARED PHOTOMETRY OF GLOBULAR CLUSTERS IN NGC 1399: EVIDENCE FOR COLOR-METALLICITY NONLINEARITY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Fornax Cluster; Bimodality; Photometry (optics); Galaxy; Luminosity; Unimodality; Apparent magnitude","score_opus":0.021165836952173007,"score_gpt":0.2725423757691712,"score_spread":0.2513765388169982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021631795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99896085,0.000022953644,0.000111908805,0.000012173139,0.0000014512062,0.0000027962863,0.00016295699,0.00001024481,0.00071476534],"genre_scores_gemma":[0.99903905,0.000018030618,0.00022988404,0.000007969314,0.000004050868,0.0000033168994,0.00054272613,0.000008266079,0.0001466685],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997446,0.000018721938,0.000017531618,0.00008472696,0.00009218768,0.000042233693],"domain_scores_gemma":[0.9994429,0.00006320586,0.00018117393,0.000057929425,0.00008694877,0.00016784445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028479044,0.00023362783,0.00024326926,0.0013118627,0.0004408067,0.00048630335,0.0003985353,0.00024877457,0.0010134479],"category_scores_gemma":[0.0009012024,0.0002002098,0.0002762037,0.00078404974,0.00037422316,0.00040715915,0.00085568905,0.00022693796,0.00032501973],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014956667,0.000028669812,0.9666767,0.000010432462,0.00004746132,0.000073005045,0.00016218578,0.000304717,0.029161457,0.00018300053,0.00013905215,0.0030637633],"study_design_scores_gemma":[0.000004344991,0.000012019019,0.9986546,0.0000017877169,0.0000067518963,0.00005098468,0.000050334787,0.0005636226,0.00045185824,0.000083715044,0.00011664034,0.0000032333542],"about_ca_topic_score_codex":0.017286254,"about_ca_topic_score_gemma":0.031314407,"teacher_disagreement_score":0.017286254,"about_ca_system_score_codex":0.0006800396,"about_ca_system_score_gemma":0.000253337,"threshold_uncertainty_score":0.034371257},"labels":[],"label_agreement":null},{"id":"W2021723259","doi":"10.1088/0004-637x/751/1/74","title":"THE RECENT STELLAR ARCHEOLOGY OF M31—THE NEAREST RED DISK GALAXY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Stars; Galaxy; myr; Star formation; Spiral galaxy; Astronomy; Luminosity; Chemistry","score_opus":0.011262018953862777,"score_gpt":0.22481611909433877,"score_spread":0.213554100140476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021723259","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92705935,0.021040509,0.0016694046,0.0049483487,0.000527012,0.000016798458,0.0002889749,0.0000533015,0.04439617],"genre_scores_gemma":[0.99153143,0.0031696137,0.0002913186,0.0002477281,0.00052319665,0.0000020850594,0.00018774784,0.000010550885,0.0040363795],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999,0.000013467799,0.0000051033776,0.000035402074,0.000023350276,0.000022698634],"domain_scores_gemma":[0.99932337,0.00008502144,0.0001399329,0.00007767551,0.00020452634,0.00016938764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007066696,0.00013515467,0.00018812719,0.00090306293,0.00081861665,0.0012417134,0.0002815991,0.0005633096,0.0024747353],"category_scores_gemma":[0.0011695086,0.0000734493,0.00014444871,0.0007539985,0.0006781265,0.0009424691,0.0007399248,0.00050426094,0.0005435655],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084056484,0.00013979046,0.4911424,0.000854876,0.00016479439,0.0022627423,0.006298254,0.002934282,0.058852687,0.05529542,0.01717859,0.36403552],"study_design_scores_gemma":[0.000009040495,0.00012562987,0.9128175,0.00007938972,0.00003528378,0.0011085582,0.001194897,0.0006723398,0.001108565,0.0049963985,0.07783128,0.000021098345],"about_ca_topic_score_codex":0.002715711,"about_ca_topic_score_gemma":0.004978595,"teacher_disagreement_score":0.002715711,"about_ca_system_score_codex":0.00096844276,"about_ca_system_score_gemma":0.0002997989,"threshold_uncertainty_score":0.008278787},"labels":[],"label_agreement":null},{"id":"W2021729861","doi":"10.1086/497562","title":"Keck Deep Fields. I. Observations, Reductions, and the Selection of Faint Star‐forming Galaxies at Redshifts<i>z</i>∼ 4, 3, and 2","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Redshift; Galaxy; Sky; Luminosity; Luminosity function; Galaxy formation and evolution; Hubble Deep Field; Selection (genetic algorithm)","score_opus":0.008269595403574005,"score_gpt":0.20288223376344344,"score_spread":0.19461263835986944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021729861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.63996154,0.0049522617,0.030825583,0.0010180502,0.00017107825,0.00092442933,0.26890326,0.003317209,0.049926676],"genre_scores_gemma":[0.60188293,0.0032758398,0.086411774,0.0013646216,0.0002132992,0.0012515355,0.27286384,0.0007215974,0.03201461],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995334,0.000041411502,0.000035899047,0.00016539739,0.00011914366,0.00010477215],"domain_scores_gemma":[0.99891126,0.00010548471,0.00032070468,0.00028667564,0.00015032185,0.00022564047],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007737269,0.00066658284,0.00035897284,0.0041453736,0.0006395427,0.0007118498,0.00057976117,0.0002871187,0.004849122],"category_scores_gemma":[0.0012480773,0.00054744823,0.00029793603,0.0025064237,0.00032548702,0.001040331,0.0013664211,0.0005206192,0.002758261],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089150347,0.00029736926,0.5341355,0.00085239817,0.00019148731,0.00034450955,0.001030263,0.0020790081,0.04331813,0.008770799,0.12116189,0.2869271],"study_design_scores_gemma":[0.00007322527,0.000066351786,0.8674837,0.00010018344,0.000060713697,0.00038707067,0.00018612281,0.0006084363,0.0073816194,0.0020347696,0.12157506,0.00004278078],"about_ca_topic_score_codex":0.01015709,"about_ca_topic_score_gemma":0.019463755,"teacher_disagreement_score":0.01015709,"about_ca_system_score_codex":0.0010523284,"about_ca_system_score_gemma":0.0006215593,"threshold_uncertainty_score":0.020195901},"labels":[],"label_agreement":null},{"id":"W2021759142","doi":"10.1086/429128","title":"The Mean Pulse Profile of PSR J0737-3039A","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Millisecond pulsar; Orbit (dynamics); General relativity; Pulse (music); Telescope; Spin (aerodynamics); Beam (structure)","score_opus":0.010587595137674419,"score_gpt":0.3086664843162876,"score_spread":0.2980788891786132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021759142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969971,0.00010129224,0.0005647047,0.000041541203,0.000008334411,0.0000046700525,0.0008005005,0.00005617518,0.0014256617],"genre_scores_gemma":[0.997241,0.000047470214,0.00054110645,0.000016232936,0.000008073449,0.0000063983903,0.0016976376,0.0000143090365,0.0004276993],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993527,0.000005953772,0.000004414475,0.00001972733,0.000021621732,0.000013109291],"domain_scores_gemma":[0.9997297,0.00003979517,0.000058117283,0.000034501918,0.000074208896,0.000063559884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019035088,0.00011544578,0.00020250154,0.00048164374,0.00036825123,0.00026479067,0.00016660606,0.00022337248,0.0013028204],"category_scores_gemma":[0.00049594184,0.000104689025,0.00012039865,0.00049663964,0.00014451609,0.00020072839,0.00021029395,0.00027911406,0.00074571586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005791289,0.00015419927,0.6860986,0.000108977205,0.00012018262,0.0006238716,0.0004567549,0.0024154314,0.25383657,0.0015600242,0.0041084876,0.049937725],"study_design_scores_gemma":[0.000009314091,0.00009191109,0.9852557,0.000005145059,0.000017002036,0.0006639483,0.000065258806,0.0031257025,0.008406103,0.00028095974,0.0020611242,0.0000176745],"about_ca_topic_score_codex":0.0031214738,"about_ca_topic_score_gemma":0.004744436,"teacher_disagreement_score":0.0031214738,"about_ca_system_score_codex":0.00030311497,"about_ca_system_score_gemma":0.00018566973,"threshold_uncertainty_score":0.006206572},"labels":[],"label_agreement":null},{"id":"W2021782408","doi":"10.1086/432876","title":"Toward an Empirical Determination of the ZZ Ceti Instability Strip","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Instability strip; White dwarf; Stars; Astrophysics; Surface gravity; Physics; Sky; Effective temperature; Stellar classification; Instability; Spectral line; Homogeneous; Astronomy","score_opus":0.027236308699601794,"score_gpt":0.2744516336318052,"score_spread":0.24721532493220338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021782408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9733358,0.00045893207,0.021986704,0.00008370473,0.0000062139648,0.000020866159,0.00059138687,0.00022840573,0.0032879196],"genre_scores_gemma":[0.99128,0.00015397758,0.007489066,0.000028942792,0.000015922293,0.000012003635,0.0007948895,0.00003361222,0.00019160847],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959344,0.000058254733,0.000031001826,0.00017016307,0.00010548932,0.00004168085],"domain_scores_gemma":[0.99685234,0.00093872624,0.0010492776,0.00057208515,0.000386481,0.00020116007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009892484,0.00032026225,0.00033006776,0.0031102397,0.00039866753,0.0013786166,0.00044109375,0.000229739,0.0006326006],"category_scores_gemma":[0.0037401987,0.00019235365,0.00023537,0.0017097335,0.0004287016,0.00048980204,0.0012113232,0.00057371147,0.000394138],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007573902,0.000018321905,0.9584306,0.000033956643,0.00004557255,0.00008488882,0.00032203778,0.0015288786,0.0139317745,0.0016083533,0.0002672515,0.023652544],"study_design_scores_gemma":[0.000010891587,0.000050830622,0.96184564,0.000019368861,0.00003269956,0.0003113842,0.00029561055,0.02415836,0.008045853,0.0032709606,0.0019434724,0.000014885672],"about_ca_topic_score_codex":0.0011564284,"about_ca_topic_score_gemma":0.001141987,"teacher_disagreement_score":0.0031102397,"about_ca_system_score_codex":0.00023666618,"about_ca_system_score_gemma":0.00016387047,"threshold_uncertainty_score":0.0052316785},"labels":[],"label_agreement":null},{"id":"W2021857340","doi":"10.1088/0004-637x/770/2/141","title":"HIERARCHICAL STRUCTURE OF MAGNETOHYDRODYNAMIC TURBULENCE IN POSITION-POSITION-VELOCITY SPACE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Magnetohydrodynamic turbulence; Mach number; Magnetohydrodynamic drive; Turbulence; Magnetohydrodynamics; Supersonic speed; Dendrogram; Space (punctuation)","score_opus":0.0034858431578125575,"score_gpt":0.2081878161931302,"score_spread":0.20470197303531765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021857340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97073495,0.00007725951,0.02756857,0.00006569999,0.0000063414354,0.000018801906,0.0003154511,0.00017168582,0.0010412344],"genre_scores_gemma":[0.9907919,0.00003501429,0.008562494,0.000010201494,0.0000036078918,0.000013673271,0.00036725204,0.000027140159,0.00018877529],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998703,0.00002877092,0.000009267587,0.000028141536,0.000029525563,0.000033910226],"domain_scores_gemma":[0.9991316,0.00032198022,0.00022329074,0.00006272257,0.00015900643,0.00010133354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020560181,0.00014252044,0.00015513659,0.0012562482,0.00042406644,0.0007449949,0.00021795217,0.00019739456,0.0006499289],"category_scores_gemma":[0.0013700807,0.0001403465,0.0002795844,0.00075759355,0.0004118361,0.00054341945,0.00041774742,0.00024872762,0.000087970184],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005274674,0.00023351186,0.18200807,0.00022102347,0.0001696905,0.0008662996,0.0025341175,0.5498841,0.12026105,0.08739181,0.0028421606,0.05306079],"study_design_scores_gemma":[0.000021150818,0.00006394979,0.07510159,0.000018383635,0.000020005684,0.00013175928,0.0003001544,0.89373887,0.0069849575,0.022122597,0.0014602001,0.00003642012],"about_ca_topic_score_codex":0.003037929,"about_ca_topic_score_gemma":0.0030222938,"teacher_disagreement_score":0.003037929,"about_ca_system_score_codex":0.000594538,"about_ca_system_score_gemma":0.0003375293,"threshold_uncertainty_score":0.0060405135},"labels":[],"label_agreement":null},{"id":"W2021926159","doi":"10.1088/0004-637x/770/1/61","title":"THE IMACS CLUSTER BUILDING SURVEY. I. DESCRIPTION OF THE SURVEY AND ANALYSIS METHODS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Photometry (optics); Supercluster (genetic); Astronomy; Spectrograph; Cluster (spacecraft); Redshift; Galaxy cluster; Luminous infrared galaxy; Star formation; Star cluster; Stars; Spectral line; Computer science","score_opus":0.01871022363922458,"score_gpt":0.2676651585552224,"score_spread":0.2489549349159978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021926159","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.020032994,0.0005972348,0.018375598,0.0007509751,0.0001460851,0.007894809,0.9135795,0.0031302182,0.035492472],"genre_scores_gemma":[0.029335544,0.00064679893,0.07627603,0.0005632747,0.0002467007,0.017594181,0.85717076,0.0010648048,0.017102001],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9966293,0.00083504454,0.00032305566,0.0006124132,0.0011686757,0.00043147456],"domain_scores_gemma":[0.99540126,0.0003780789,0.00071866193,0.0012937551,0.0016482144,0.0005600063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0036762008,0.0013138095,0.0010480044,0.010387908,0.0014209768,0.0017800708,0.0041700206,0.0008076002,0.030267052],"category_scores_gemma":[0.0046562967,0.0007931492,0.00066508754,0.014559846,0.00041979854,0.0010749113,0.0027320709,0.0009385594,0.03310702],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030927447,0.00041393316,0.14704755,0.0009808707,0.00018084193,0.00013981486,0.0007063495,0.0040917313,0.0018747179,0.008092073,0.7116144,0.12454837],"study_design_scores_gemma":[0.00014191018,0.00010413904,0.255841,0.00018500212,0.000054022454,0.00021209342,0.00057139783,0.0028493812,0.0015581868,0.0022741677,0.7361011,0.000107616535],"about_ca_topic_score_codex":0.056138854,"about_ca_topic_score_gemma":0.048876483,"teacher_disagreement_score":0.056138854,"about_ca_system_score_codex":0.002157419,"about_ca_system_score_gemma":0.0029025008,"threshold_uncertainty_score":0.11162418},"labels":[],"label_agreement":null},{"id":"W2021934314","doi":"10.1086/444618","title":"The Dependence of Galaxy Colors on Luminosity and Environment at <i>z</i> ~ 0.4","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Brightest cluster galaxy; Luminous infrared galaxy; Lenticular galaxy; Astronomy; Elliptical galaxy; Luminosity function; Interacting galaxy; Peculiar galaxy; Galaxy; Sky; Redshift; Galaxy merger; Luminosity; Galaxy group; Galaxy cluster; Galaxy formation and evolution; Surface brightness fluctuation","score_opus":0.005506694641242147,"score_gpt":0.1894203930367082,"score_spread":0.18391369839546606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021934314","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99707353,0.000060148166,0.00054720865,0.000045449782,0.0000013543485,0.0000026165494,0.0003484834,0.000042355492,0.0018787987],"genre_scores_gemma":[0.99879336,0.000036470334,0.000268569,0.000012199221,0.0000038787553,0.0000020257094,0.00044043968,0.000012991552,0.0004299303],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985874,0.000019448542,0.0000036641484,0.000033483975,0.000025844472,0.000058799505],"domain_scores_gemma":[0.99790406,0.0007710663,0.00058260566,0.00013298781,0.00029748242,0.00031176957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029740107,0.00021976786,0.00013347474,0.00095069234,0.00024278708,0.00082392845,0.0003097467,0.00029869995,0.0020223756],"category_scores_gemma":[0.0020705645,0.0002159377,0.0003292823,0.0006588987,0.0003282452,0.00040442866,0.00040300487,0.000262497,0.0004791609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001539626,0.000025207615,0.98418033,0.000013322542,0.00006543385,0.00009316182,0.00011204554,0.0028972768,0.0055338414,0.0006144067,0.00038963853,0.005921418],"study_design_scores_gemma":[0.000003046478,0.0000330855,0.99537164,0.0000015889068,0.000016704656,0.000055264198,0.000056270084,0.0030007064,0.000943105,0.00017231575,0.00034222112,0.000004060207],"about_ca_topic_score_codex":0.008223831,"about_ca_topic_score_gemma":0.013777445,"teacher_disagreement_score":0.008223831,"about_ca_system_score_codex":0.0005169915,"about_ca_system_score_gemma":0.00011049963,"threshold_uncertainty_score":0.016351938},"labels":[],"label_agreement":null},{"id":"W2021960159","doi":"10.1086/509570","title":"Methanol in the L1551 Circumbinary Torus","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Planetesimal; Circumbinary planet; Astrophysics; Torus; Physics; Astronomy; Stars; Solar System; Geometry","score_opus":0.009324789277826607,"score_gpt":0.23552584092751944,"score_spread":0.22620105164969284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2021960159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99840087,0.00022674212,0.00007526978,0.000016857623,0.0000035163516,0.0000026418463,0.00009433449,0.000017590579,0.0011620478],"genre_scores_gemma":[0.99935013,0.000064378626,0.00015430732,0.000015566335,0.0000055107903,0.000002317532,0.00019580733,0.0000048102147,0.00020712818],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999467,0.0000024162373,0.0000016274845,0.000019407673,0.000010532093,0.000019295596],"domain_scores_gemma":[0.99991286,0.000009081489,0.00003469716,0.000009393431,0.000009023793,0.000024902569],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000068393645,0.00019622456,0.0002095032,0.00042983843,0.000542201,0.00054581667,0.00037478883,0.00025802903,0.00096063066],"category_scores_gemma":[0.00014696298,0.00014878712,0.00009830702,0.00028657005,0.00027417534,0.00031524478,0.00053536624,0.00017174293,0.00034164242],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096781267,0.00014990725,0.3175581,0.00017401508,0.00013382977,0.004271697,0.0014229106,0.002605533,0.6519471,0.00081223395,0.0013097563,0.018647086],"study_design_scores_gemma":[0.000056366618,0.00022683253,0.95836335,0.00002832943,0.00006802336,0.001095356,0.0008548904,0.0028446238,0.03196978,0.0003412365,0.0041256165,0.000025558995],"about_ca_topic_score_codex":0.003388015,"about_ca_topic_score_gemma":0.0036170322,"teacher_disagreement_score":0.003388015,"about_ca_system_score_codex":0.00051581877,"about_ca_system_score_gemma":0.00010773895,"threshold_uncertainty_score":0.0067365766},"labels":[],"label_agreement":null},{"id":"W2022042621","doi":"10.1086/509784","title":"A New View of the Dwarf Spheroidal Satellites of the Milky Way from VLT FLAMES: Where Are the Very Metal-poor Stars?","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":211,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Milky Way; Metallicity; Dwarf galaxy; Galaxy; Stars; Dwarf spheroidal galaxy","score_opus":0.010155673917230403,"score_gpt":0.23426955647713754,"score_spread":0.22411388255990713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022042621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96099865,0.012826958,0.004082382,0.008193207,0.0001460888,0.0000072672046,0.0002262001,0.00011510929,0.013404183],"genre_scores_gemma":[0.9911329,0.0025060885,0.0017477365,0.0014760948,0.00021579812,0.000003507188,0.0001810311,0.000023111663,0.0027138551],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998994,0.000010077708,0.0000072657162,0.000029648885,0.00002793885,0.00002572807],"domain_scores_gemma":[0.99946624,0.00007622297,0.00015150222,0.00008465226,0.00009671142,0.00012461233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032063437,0.00019314907,0.00033179508,0.0012417785,0.00068862643,0.0022092094,0.0004822042,0.0007433578,0.001294939],"category_scores_gemma":[0.00082163484,0.00020922453,0.00018399674,0.00066334795,0.0021665515,0.004348898,0.0011387456,0.0008983061,0.00030816233],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005153526,0.000095272466,0.66776645,0.0005873612,0.0001286855,0.0034392553,0.014280555,0.001009071,0.07471931,0.060394295,0.00566987,0.17139444],"study_design_scores_gemma":[0.000046451933,0.00022581324,0.75664383,0.00026853607,0.00012661806,0.005868274,0.014708501,0.002297727,0.008051597,0.06840945,0.14325732,0.00009589167],"about_ca_topic_score_codex":0.0043528755,"about_ca_topic_score_gemma":0.011081996,"teacher_disagreement_score":0.0043528755,"about_ca_system_score_codex":0.00065770285,"about_ca_system_score_gemma":0.00041023738,"threshold_uncertainty_score":0.008655071},"labels":[],"label_agreement":null},{"id":"W2022214574","doi":"10.1086/529507","title":"Analysis of the<i>FUSE</i>Spectrum of the Hot, Evolved Star GD 6051","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Spectral line; Balmer series; Effective temperature; Line (geometry); Ionization; Stellar atmosphere; Helium; Atmosphere (unit); Instability strip; Stars; Ion; Astronomy; Emission spectrum; Atomic physics","score_opus":0.010372808549232122,"score_gpt":0.20566945793302513,"score_spread":0.19529664938379301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022214574","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99755067,0.00006477493,0.0003540187,0.000019300775,0.0000029137977,0.0000027757078,0.00079659413,0.000050168837,0.001158748],"genre_scores_gemma":[0.99805474,0.00002690732,0.00046118774,0.000015383323,0.0000032161229,0.0000017869464,0.0013278755,0.000008861651,0.000100037294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999949,0.0000035781375,0.000003084074,0.000019450112,0.000014567474,0.0000102992935],"domain_scores_gemma":[0.9998981,0.000018494524,0.000030398644,0.000015433368,0.000015490583,0.0000221384],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009904481,0.00023359532,0.0001371438,0.0007486463,0.00021614491,0.0002788946,0.00017243883,0.00023420615,0.00045662833],"category_scores_gemma":[0.00019740379,0.00008302205,0.00033255102,0.00044370838,0.00013080821,0.00015241768,0.00018967818,0.00012210204,0.00010083738],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012271332,0.00021402411,0.5089039,0.00021253178,0.00048154485,0.0020884296,0.0006959245,0.026502281,0.41502225,0.0015258512,0.002191145,0.04093497],"study_design_scores_gemma":[0.000014385039,0.000075992066,0.9737181,0.000009314574,0.00006469197,0.00028663353,0.00008334434,0.014712815,0.009572328,0.0001436351,0.0013043269,0.000014343217],"about_ca_topic_score_codex":0.007413765,"about_ca_topic_score_gemma":0.007549791,"teacher_disagreement_score":0.007413765,"about_ca_system_score_codex":0.00047809602,"about_ca_system_score_gemma":0.0000742185,"threshold_uncertainty_score":0.014741242},"labels":[],"label_agreement":null},{"id":"W2022225992","doi":"10.1086/321739","title":"Star Formation, Supernova Feedback, and the Angular Momentum Problem in Numerical Cold Dark Matter Cosmogony: Halfway There?","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Angular momentum; Supernova; Galaxy; Cold dark matter; Dark matter; Redshift; Baryon; Specific relative angular momentum","score_opus":0.007556468577838785,"score_gpt":0.23057887304054678,"score_spread":0.223022404462708,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022225992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9506429,0.0017522387,0.032224778,0.008238492,0.00026195322,0.000024427845,0.00011385117,0.00042763483,0.0063135996],"genre_scores_gemma":[0.98728555,0.0005406017,0.010075666,0.0003166522,0.00010200989,0.000022573713,0.00004000514,0.00013453895,0.0014823291],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997646,0.00014317305,0.000011293664,0.000020132173,0.00002764818,0.000033142805],"domain_scores_gemma":[0.99830437,0.0010188938,0.00020136933,0.00016078896,0.00008244328,0.00023209673],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013005603,0.00039448385,0.0005898466,0.00027526257,0.0009101319,0.0015136128,0.001023765,0.0016136443,0.0020005684],"category_scores_gemma":[0.008030943,0.00046048517,0.00037910073,0.0004165652,0.0024816333,0.0029615248,0.0016584678,0.0011140355,0.00017148307],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051968195,0.00020843424,0.02851167,0.00015762549,0.00015137545,0.00039751362,0.0006326625,0.8001461,0.00152837,0.14420241,0.0038254443,0.019718723],"study_design_scores_gemma":[0.00012961039,0.00003704486,0.0012368076,0.000014399917,0.000020405585,0.000030490732,0.00009539388,0.9533078,0.00035320807,0.04392912,0.00082782866,0.000018024188],"about_ca_topic_score_codex":0.015145885,"about_ca_topic_score_gemma":0.010779593,"teacher_disagreement_score":0.015145885,"about_ca_system_score_codex":0.0006595898,"about_ca_system_score_gemma":0.00076797453,"threshold_uncertainty_score":0.030115485},"labels":[],"label_agreement":null},{"id":"W2022340545","doi":"10.1086/511175","title":"Testing Models of Radio Galaxy Evolution and the Cosmological Impact of FR II Radio Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Quasar; Galaxy; X-shaped radio galaxy; Radio galaxy; Spectral index; Redshift; RADIUS; Galaxy formation and evolution","score_opus":0.013851198394255743,"score_gpt":0.23138029609750674,"score_spread":0.217529097703251,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022340545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9896047,0.00011572981,0.007256595,0.00027837857,0.000008685458,0.000019342164,0.00019699751,0.00005993086,0.0024596045],"genre_scores_gemma":[0.99775994,0.0000755609,0.0016973793,0.00003788532,0.000014177988,0.000013093403,0.00016148877,0.000013679578,0.00022677689],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99815816,0.0010889827,0.000074563766,0.00032676818,0.00012778743,0.00022368095],"domain_scores_gemma":[0.96584076,0.027834836,0.0033982727,0.0013369197,0.00073034945,0.00085895153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005785927,0.0013719094,0.0005823777,0.0010662865,0.0005031533,0.0020371713,0.0018939052,0.001063325,0.002728869],"category_scores_gemma":[0.023660714,0.00038796457,0.001296718,0.001012821,0.0014088557,0.0015875953,0.0009812303,0.0007515853,0.00031308498],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087804085,0.0003961339,0.43863732,0.00012561094,0.0008415986,0.00048420843,0.0006661359,0.52088606,0.0026768635,0.020268774,0.0007291811,0.013410009],"study_design_scores_gemma":[0.0001314473,0.0007202323,0.08417346,0.000021783007,0.0002697391,0.00018775754,0.0004719639,0.89879316,0.0018139615,0.012709825,0.0006478111,0.000058872367],"about_ca_topic_score_codex":0.020593429,"about_ca_topic_score_gemma":0.0075344187,"teacher_disagreement_score":0.020593429,"about_ca_system_score_codex":0.0019448114,"about_ca_system_score_gemma":0.0006254039,"threshold_uncertainty_score":0.04094714},"labels":[],"label_agreement":null},{"id":"W2022625885","doi":"10.1088/0004-637x/743/1/90","title":"THE FIRST PUBLIC RELEASE OF SOUTH POLE TELESCOPE DATA: MAPS OF A 95 deg<sup>2</sup>FIELD FROM 2008 OBSERVATIONS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; South Pole Telescope; Sky; Cosmic microwave background; Telescope; Galaxy; Astronomy; Astrophysics; Pipeline (software); Remote sensing; Galaxy cluster; Optics; Geography; Computer science","score_opus":0.03347261363287508,"score_gpt":0.21297957500297954,"score_spread":0.17950696137010447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022625885","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01030339,0.000108756845,0.0026930443,0.00030794565,0.0001358402,0.0001770121,0.96040046,0.006096746,0.01977684],"genre_scores_gemma":[0.010997536,0.00011313678,0.01011181,0.00018151611,0.00009256826,0.00027795718,0.9685016,0.0016850717,0.0080387015],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9995084,0.000020799569,0.000027963479,0.00007290888,0.00030073238,0.000069118854],"domain_scores_gemma":[0.9977608,0.00020824448,0.00032498722,0.00068293436,0.0007834224,0.00023961594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053462916,0.0005626316,0.00045719868,0.0020371326,0.0004903584,0.0013267492,0.0011310822,0.0006620823,0.057004098],"category_scores_gemma":[0.0024097885,0.0005974635,0.00036991216,0.0031878734,0.00020677017,0.00091809034,0.0011562658,0.0009420679,0.052334536],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023225581,0.00004961985,0.008494463,0.00024633293,0.0000316148,0.0001465603,0.00015950062,0.00034409546,0.0047808746,0.0005203901,0.9462736,0.038720712],"study_design_scores_gemma":[0.00014000523,0.000039064544,0.108511575,0.000054121614,0.000025385456,0.00013399175,0.00009316873,0.00056626246,0.0024197113,0.0004722113,0.8875146,0.000029839464],"about_ca_topic_score_codex":0.017642446,"about_ca_topic_score_gemma":0.027728928,"teacher_disagreement_score":0.057004098,"about_ca_system_score_codex":0.00078476244,"about_ca_system_score_gemma":0.0011898448,"threshold_uncertainty_score":0.19069767},"labels":[],"label_agreement":null},{"id":"W2022630763","doi":"10.1086/505294","title":"Dynamical H<scp>ii</scp>Region Evolution in Turbulent Molecular Clouds","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Ionization; Turbulence; Physics; Photoablation; H II region; Time evolution; Molecular cloud; Star formation; Astrophysics; Mechanics; Atomic physics; Computational physics; Optics; Laser; Galaxy; Ion; Stars","score_opus":0.004856553275297738,"score_gpt":0.20924641208033853,"score_spread":0.2043898588050408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022630763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996888,0.000039219747,0.0015629367,0.00008584388,0.000010003462,0.000011263221,0.000087995846,0.00006482642,0.0012499107],"genre_scores_gemma":[0.99880195,0.000023448394,0.00083367096,0.000018368488,0.0000052897612,0.000009423959,0.000095552416,0.000014998459,0.00019742582],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990654,0.000022037604,0.0000048070074,0.0000136289555,0.000016768507,0.000036166028],"domain_scores_gemma":[0.99951124,0.00016384735,0.00009721883,0.000026818172,0.000055200293,0.00014565383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002630559,0.00040762112,0.0003651259,0.00041434314,0.0005730901,0.0007857022,0.00071252615,0.0005916596,0.00076001376],"category_scores_gemma":[0.0012993532,0.00032846368,0.00047006164,0.00042130833,0.00094748,0.00050406245,0.0005235431,0.0004938455,0.00009178237],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020072299,0.000087158296,0.012382371,0.00001665747,0.00006115614,0.00024088274,0.0001176237,0.9781788,0.0047000223,0.0028598637,0.00021254261,0.0009421556],"study_design_scores_gemma":[0.00005603592,0.00004823711,0.002729741,0.0000027580631,0.000011722389,0.00001641221,0.000034408506,0.99607074,0.00056278444,0.0003643386,0.00009342219,0.000009331814],"about_ca_topic_score_codex":0.029014336,"about_ca_topic_score_gemma":0.012371542,"teacher_disagreement_score":0.029014336,"about_ca_system_score_codex":0.0016925322,"about_ca_system_score_gemma":0.0006630575,"threshold_uncertainty_score":0.05769092},"labels":[],"label_agreement":null},{"id":"W2022692747","doi":"10.1088/0004-637x/716/2/1118","title":"SUNYAEV–ZEL’DOVICH CLUSTER PROFILES MEASURED WITH THE SOUTH POLE TELESCOPE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":150,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Cluster (spacecraft); South Pole Telescope; Virial theorem; Galaxy cluster; RADIUS; Observable; Sunyaev–Zel'dovich effect; Telescope; Galaxy; Virial mass","score_opus":0.006220072727145839,"score_gpt":0.19713575722759052,"score_spread":0.1909156845004447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022692747","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99841,0.000021345271,0.00026051002,0.000009996583,8.95451e-7,0.0000019320596,0.00028247043,0.000021217187,0.0009915433],"genre_scores_gemma":[0.9993149,0.000009404947,0.0001337292,0.0000029653702,0.0000013330314,0.0000021673397,0.00034472544,0.000004449939,0.00018645903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999318,0.0000048508514,0.0000018559876,0.000023186918,0.000022167056,0.000016108017],"domain_scores_gemma":[0.99981564,0.000018841309,0.000059610793,0.000019906462,0.000024826095,0.00006123336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009543384,0.00016521693,0.00022812137,0.0005046899,0.00030508442,0.00030155617,0.00022242442,0.00010942267,0.0011374257],"category_scores_gemma":[0.00024179097,0.00014509725,0.00013041701,0.00028560287,0.00018516147,0.000115840994,0.00042772564,0.00011899589,0.00020251585],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029938738,0.00001949475,0.9449014,0.000022896025,0.0000907923,0.00014200104,0.00053311244,0.0037814525,0.04188429,0.00060930284,0.0011217844,0.006593942],"study_design_scores_gemma":[0.0000032326484,0.000008966332,0.99726605,8.317089e-7,0.0000038189787,0.000022340037,0.000025645535,0.0013928659,0.0009531172,0.000028308728,0.00029251236,0.000002348563],"about_ca_topic_score_codex":0.0092150755,"about_ca_topic_score_gemma":0.010151137,"teacher_disagreement_score":0.0092150755,"about_ca_system_score_codex":0.0005876449,"about_ca_system_score_gemma":0.00011046013,"threshold_uncertainty_score":0.018322885},"labels":[],"label_agreement":null},{"id":"W2022706188","doi":"10.1088/0004-637x/776/2/127","title":"CHROMOSPHERICALLY ACTIVE STARS IN THE RADIAL VELOCITY EXPERIMENT (RAVE) SURVEY. I. THE CATALOG","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Stars; Astrophysics; Physics; Radial velocity; Spectral line; Metallicity; Emission spectrum; Flux (metallurgy); Sky; Equivalent width; Line (geometry); Astronomy; Geometry","score_opus":0.013947390151028772,"score_gpt":0.23243406215088314,"score_spread":0.21848667199985436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022706188","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8693905,0.0012044504,0.0014170958,0.00009044075,0.000040800813,0.000084940155,0.12094384,0.00049946486,0.006328419],"genre_scores_gemma":[0.6551101,0.00067391427,0.0042725056,0.00012152718,0.00005756864,0.00010157938,0.33502966,0.00011130689,0.0045217657],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996619,0.000042869466,0.000042100914,0.00011026681,0.00008410902,0.000058775036],"domain_scores_gemma":[0.9992317,0.000071904295,0.00020362638,0.00014234663,0.00016749433,0.00018296728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00070500706,0.00026877815,0.0003590543,0.002636022,0.00026912714,0.00051968097,0.0002807763,0.00022609308,0.0027231756],"category_scores_gemma":[0.0009759389,0.00013955886,0.0002503266,0.0019069985,0.00010606242,0.00035165847,0.0005753658,0.00019150012,0.003257558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018828663,0.000067895824,0.94096977,0.0001065256,0.000106410254,0.00012128155,0.00024448638,0.00026495883,0.002896887,0.0005195762,0.02398032,0.030533565],"study_design_scores_gemma":[0.000018582177,0.000048256865,0.9702331,0.000020545109,0.000029449164,0.00025349233,0.00013790159,0.00054497947,0.00052577676,0.00011576375,0.028067213,0.000005095602],"about_ca_topic_score_codex":0.0035700188,"about_ca_topic_score_gemma":0.0055463314,"teacher_disagreement_score":0.0035700188,"about_ca_system_score_codex":0.00017107592,"about_ca_system_score_gemma":0.0003196546,"threshold_uncertainty_score":0.009109974},"labels":[],"label_agreement":null},{"id":"W2022790250","doi":"10.1088/0004-637x/732/1/29","title":"AFTERGLOW OBSERVATIONS OF<i>FERMI</i>LARGE AREA TELESCOPE GAMMA-RAY BURSTS AND THE EMERGING CLASS OF HYPER-ENERGETIC EVENTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":195,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico; U.S. Department of Energy; Consejo Nacional de Investigaciones Científicas y Técnicas; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Gamma-ray burst; Fermi Gamma-ray Space Telescope; Afterglow; Astrophysics; Redshift; Magnetar; Light curve; Jet (fluid); Kinetic energy; Lorentz factor; Astrophysical jet; Astronomy; Galaxy; Active galactic nucleus; Neutron star; Lorentz transformation","score_opus":0.021429790966709914,"score_gpt":0.2216439297518519,"score_spread":0.200214138785142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022790250","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97935355,0.000876623,0.00063067337,0.00039136194,0.00003994298,0.000009459482,0.0010987344,0.000065386244,0.017534308],"genre_scores_gemma":[0.9959352,0.0004086586,0.00035604378,0.00009451768,0.000043970234,0.000005151971,0.0009091007,0.00001591895,0.002231431],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989986,0.000011821105,0.0000059139666,0.000025577285,0.000027441809,0.000029308789],"domain_scores_gemma":[0.9993567,0.00006767003,0.00029332328,0.00009181672,0.0000808762,0.000109590066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026369424,0.000105450985,0.00009384276,0.0012529667,0.00046054882,0.0010145763,0.00017345563,0.00032784362,0.0022738392],"category_scores_gemma":[0.0007638023,0.00006487877,0.00009269793,0.0015348573,0.00029324784,0.0004442093,0.0005988169,0.0003256509,0.0002524232],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003806787,0.00010620509,0.8754326,0.00008185929,0.000079771395,0.00046685367,0.001994861,0.00025059382,0.027785007,0.0066280114,0.006339308,0.080454245],"study_design_scores_gemma":[0.000006031069,0.000024208399,0.9849162,0.00001826243,0.00001236214,0.00021072043,0.00047133485,0.00014543766,0.0007955862,0.00071119604,0.012682886,0.0000058131245],"about_ca_topic_score_codex":0.008002219,"about_ca_topic_score_gemma":0.021852298,"teacher_disagreement_score":0.008002219,"about_ca_system_score_codex":0.0004997043,"about_ca_system_score_gemma":0.00025069367,"threshold_uncertainty_score":0.015911281},"labels":[],"label_agreement":null},{"id":"W2022792734","doi":"10.1088/0004-637x/728/2/85","title":"NEAR-INFRARED MULTI-BAND PHOTOMETRY OF THE SUBSTELLAR COMPANION GJ 758 B","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Photometry (optics); Physics; Brown dwarf; Spectral energy distribution; Astrophysics; Astronomy; Near-infrared spectroscopy; Wavelength; Stars; Spectral line; Optics","score_opus":0.024197569097782232,"score_gpt":0.22752962395293105,"score_spread":0.20333205485514882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022792734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986449,0.000047651738,0.0001060766,0.000013960144,0.000002640454,0.0000037931452,0.00021559805,0.000026528585,0.0009389351],"genre_scores_gemma":[0.9988225,0.00002295607,0.0004664356,0.000012414615,0.000004145222,0.0000032974922,0.00041598588,0.0000044696662,0.00024779674],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993956,0.0000037920836,0.000003873305,0.000021557173,0.00001716411,0.000014079413],"domain_scores_gemma":[0.9998685,0.00000878796,0.00003059312,0.000019140816,0.00002188499,0.000050983457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010550671,0.00013146432,0.0001475979,0.0011345024,0.00040018282,0.00020671713,0.0001810709,0.00022523072,0.0009149911],"category_scores_gemma":[0.00022164155,0.00008369525,0.00009375403,0.0004607139,0.00010123781,0.0001543728,0.00040460046,0.00015647155,0.00026273108],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000314903,0.00010502178,0.6815656,0.000077168675,0.00006232354,0.0013220388,0.00094050734,0.0009007168,0.2835715,0.00088838185,0.0023472435,0.027904576],"study_design_scores_gemma":[0.000003685597,0.000029649462,0.9971591,0.000003577801,0.000009660183,0.00024738713,0.00007499372,0.00033417417,0.0013409427,0.0000487307,0.0007452502,0.000002886955],"about_ca_topic_score_codex":0.007318246,"about_ca_topic_score_gemma":0.013874481,"teacher_disagreement_score":0.007318246,"about_ca_system_score_codex":0.00020270691,"about_ca_system_score_gemma":0.00007817094,"threshold_uncertainty_score":0.0145513415},"labels":[],"label_agreement":null},{"id":"W2022920666","doi":"10.1086/424375","title":"The Number Density of 0.6 &lt;<i>z</i>&lt; 1.7 Mg<scp>ii</scp>Systems from CORALS: Observational Biases at Intermediate Redshift","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Redshift; Astrophysics; Quasar; Physics; Galaxy; Equivalent width; Line (geometry); Emission spectrum; Astronomy; Spectral line; Mathematics","score_opus":0.020604978921706155,"score_gpt":0.23241497787297086,"score_spread":0.2118099989512647,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022920666","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982048,0.00015219236,0.00010990727,0.000023381403,0.0000012512376,0.000004540856,0.00038188262,0.000014506785,0.0011074004],"genre_scores_gemma":[0.9989213,0.00007481152,0.00020683662,0.000018459265,0.0000046001974,0.0000044491535,0.0005677047,0.0000057765797,0.00019616392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99947757,0.000052682622,0.00004659523,0.00015482954,0.000141464,0.00012688673],"domain_scores_gemma":[0.99831295,0.0001512414,0.00089791697,0.00016430944,0.0001846148,0.00028899676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054107606,0.00023628557,0.00022490861,0.0021835743,0.00048735627,0.0014599396,0.00053037883,0.00027735584,0.001370988],"category_scores_gemma":[0.001585731,0.00025678772,0.0002136833,0.0010739128,0.0005913955,0.00052232883,0.0009736361,0.00029137978,0.0006299612],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027356784,0.000004703968,0.99151707,0.000010826077,0.00001507357,0.000026533315,0.00021686254,0.00003853369,0.0050266967,0.00007561428,0.000082792525,0.0029579652],"study_design_scores_gemma":[0.0000010786943,0.000011087136,0.9989642,0.0000023886732,0.000010476739,0.00006588898,0.00006534425,0.000098167824,0.0005068684,0.000022808741,0.00024978496,0.0000018194141],"about_ca_topic_score_codex":0.00856656,"about_ca_topic_score_gemma":0.012476192,"teacher_disagreement_score":0.00856656,"about_ca_system_score_codex":0.00044851034,"about_ca_system_score_gemma":0.00016291667,"threshold_uncertainty_score":0.017033398},"labels":[],"label_agreement":null},{"id":"W2022998830","doi":"10.1086/426375","title":"Mass Modeling of Disk Galaxies: Degeneracies, Constraints, and Adiabatic Contraction","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Queen's University; University of British Columbia","funders":"","keywords":"Halo; Astrophysics; Physics; Galaxy rotation curve; Dark matter halo; Flattening; Galaxy; Dark matter; Cuspy halo problem; Galaxy formation and evolution; Virial theorem; Astronomy","score_opus":0.008413648761647083,"score_gpt":0.20977729926574423,"score_spread":0.20136365050409716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2022998830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95413834,0.0004426776,0.042326152,0.00016173313,0.0000056103754,0.000024036297,0.0002303574,0.00014506972,0.0025259997],"genre_scores_gemma":[0.9929524,0.00009785905,0.006448629,0.00001916315,0.000006205016,0.0000112268135,0.0002577296,0.00004916215,0.00015767831],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99903214,0.00034651512,0.00007092836,0.00024084168,0.00020803035,0.000101523874],"domain_scores_gemma":[0.9949786,0.002548492,0.0009500722,0.0010080948,0.00029353626,0.00022121471],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023397228,0.0007365692,0.00060401525,0.0009193421,0.00076141657,0.0013597142,0.0012898835,0.00059899007,0.0007267296],"category_scores_gemma":[0.01530729,0.00038008485,0.00040441978,0.00059489993,0.00069931615,0.0011591923,0.0015360152,0.00048544403,0.0002447587],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047999297,0.000082268634,0.50954974,0.00014105122,0.0001579319,0.00028240067,0.0013515172,0.39874065,0.011357521,0.020921495,0.00052447733,0.056410976],"study_design_scores_gemma":[0.000047083115,0.00010173552,0.10317224,0.00007348813,0.00004373195,0.0003068021,0.0003167925,0.8636604,0.0075014457,0.021958878,0.0027533527,0.00006412017],"about_ca_topic_score_codex":0.006355456,"about_ca_topic_score_gemma":0.0041679284,"teacher_disagreement_score":0.006355456,"about_ca_system_score_codex":0.0014443382,"about_ca_system_score_gemma":0.00059977703,"threshold_uncertainty_score":0.01263696},"labels":[],"label_agreement":null},{"id":"W2023060016","doi":"10.1088/0004-637x/717/2/1181","title":"AEGIS: A MULTIWAVELENGTH STUDY OF<i>SPITZER</i>POWER-LAW GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Redshift; Luminosity; Active galactic nucleus; Galaxy; Infrared; Power law; Astronomy; Luminous infrared galaxy","score_opus":0.0067895296952229555,"score_gpt":0.21984003374965938,"score_spread":0.21305050405443643,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023060016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988932,0.000082474515,0.000062793464,0.000018676046,6.029558e-7,0.00000536446,0.00034814025,0.0000047279877,0.00058406306],"genre_scores_gemma":[0.99794847,0.00016826259,0.00027181974,0.000017432008,0.000005603465,0.0000040749906,0.0011384164,0.000006677884,0.00043939363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998938,0.000011789723,0.0000072717617,0.00003443562,0.000021881286,0.00003074171],"domain_scores_gemma":[0.99961203,0.00004292329,0.0001844616,0.000039618204,0.00003853097,0.00008251145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016952872,0.00021980704,0.00016183581,0.0018437059,0.00024576773,0.00042197917,0.00016986446,0.00010571135,0.0010395952],"category_scores_gemma":[0.00038675722,0.00011421318,0.00020053172,0.00096170517,0.00018667057,0.00046184065,0.00043519976,0.00019467108,0.00032268345],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008032277,0.0000481264,0.98444515,0.000013850822,0.00004592446,0.0002483799,0.00048075183,0.00010781093,0.0066296286,0.00025209217,0.00037532547,0.0072725164],"study_design_scores_gemma":[0.0000015493644,0.000014391722,0.9988637,0.0000018100072,0.0000053754966,0.00019537393,0.00014589174,0.00010848828,0.00019080294,0.000019345873,0.0004520774,0.0000011343233],"about_ca_topic_score_codex":0.009927032,"about_ca_topic_score_gemma":0.014982491,"teacher_disagreement_score":0.009927032,"about_ca_system_score_codex":0.0003104166,"about_ca_system_score_gemma":0.00012238914,"threshold_uncertainty_score":0.019738495},"labels":[],"label_agreement":null},{"id":"W2023083306","doi":"10.1086/506255","title":"Quark Deconfinement in Neutron Star Cores: The Effects of Spin-down","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Deconfinement; Neutron star; Quark; Strange matter; Quark star; Stars; Neutron; Phase transition","score_opus":0.0049727301147699556,"score_gpt":0.28450959215184396,"score_spread":0.279536862037074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023083306","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99842215,0.00010926374,0.0010062344,0.00002371487,0.0000025973247,0.0000017198124,0.000007258726,0.000013653911,0.00041352585],"genre_scores_gemma":[0.9996151,0.000047024867,0.00022911042,0.000004902819,0.0000016605751,0.0000010083036,0.000010269152,0.000003856658,0.00008702522],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.999959,0.0000068504296,0.0000020038913,0.000008272728,0.0000062863132,0.000017508222],"domain_scores_gemma":[0.9995047,0.00018361729,0.00014678096,0.00003387036,0.000050168117,0.00008091594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019903884,0.000266007,0.00021246557,0.00026863007,0.00030986546,0.0003493583,0.00025437507,0.00018247776,0.00068322755],"category_scores_gemma":[0.0012265402,0.0001362547,0.0001958903,0.0001234506,0.00041119845,0.0004291017,0.00044279784,0.000295776,0.00011482996],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015606649,0.0005101762,0.13985853,0.0002236993,0.00013823625,0.0019983503,0.00068738346,0.09877986,0.7117688,0.018253127,0.00040805878,0.025813174],"study_design_scores_gemma":[0.00029927143,0.0013776078,0.10055323,0.000039211453,0.00013355607,0.0005469082,0.0002861171,0.5723146,0.3033557,0.020041954,0.0009799195,0.00007194497],"about_ca_topic_score_codex":0.0016034341,"about_ca_topic_score_gemma":0.0012922512,"teacher_disagreement_score":0.0016034341,"about_ca_system_score_codex":0.0002817876,"about_ca_system_score_gemma":0.00014678972,"threshold_uncertainty_score":0.0031881928},"labels":[],"label_agreement":null},{"id":"W2023156218","doi":"10.1086/527408","title":"Deconstructing the High‐Mass Star‐Forming Region IRAS 23033+5951","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Ultraviolet astronomy; Background radiation; Computational astrophysics; Luminosity; Stars; Astronomical spectroscopy","score_opus":0.01712575528543211,"score_gpt":0.227024772092507,"score_spread":0.20989901680707487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023156218","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8154697,0.0024820303,0.03901162,0.016181992,0.0016805648,0.00006216961,0.0009984222,0.00083039224,0.12328313],"genre_scores_gemma":[0.97912985,0.00070024346,0.0064468826,0.0005793527,0.0004512763,0.000011650812,0.00062144536,0.00033564374,0.011723785],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9996253,0.00009705067,0.0000128322035,0.00006573024,0.00014551576,0.00005350587],"domain_scores_gemma":[0.99715984,0.0006953218,0.00036134175,0.0005748889,0.0009867505,0.00022185197],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001157633,0.00027542035,0.00032563196,0.0007429754,0.00078613847,0.0022055358,0.000700052,0.0007839242,0.005955381],"category_scores_gemma":[0.008748067,0.00019692535,0.00019412355,0.0006054152,0.0010726046,0.0019913986,0.0010589845,0.0008488476,0.001680245],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005993096,0.00015691119,0.10080953,0.0007906045,0.0001442555,0.0015352885,0.004859316,0.017839119,0.038553827,0.33056998,0.06587431,0.43826768],"study_design_scores_gemma":[0.00013087843,0.00023261915,0.18593363,0.0002638917,0.00016347854,0.00092592445,0.0055041607,0.05734532,0.019239644,0.4517675,0.27835122,0.00014171265],"about_ca_topic_score_codex":0.0034347547,"about_ca_topic_score_gemma":0.0055705695,"teacher_disagreement_score":0.005955381,"about_ca_system_score_codex":0.0004039191,"about_ca_system_score_gemma":0.0011058279,"threshold_uncertainty_score":0.019922674},"labels":[],"label_agreement":null},{"id":"W2023273821","doi":"10.1088/0004-637x/757/2/133","title":"THREE NEW ECLIPSING WHITE-DWARF-M-DWARF BINARIES DISCOVERED IN A SEARCH FOR TRANSITING PLANETS AROUND M-DWARFS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; White dwarf; Astrophysics; Planet; Photometry (optics); Astronomy; Planetary system; Exoplanet; Dwarf planet; Brown dwarf; Radial velocity; Stars","score_opus":0.029280463949680542,"score_gpt":0.26148786584066114,"score_spread":0.2322074018909806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023273821","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978479,0.00010721261,0.0007952244,0.0000422187,0.000011984653,0.000022918608,0.0001379972,0.00003478202,0.0009998248],"genre_scores_gemma":[0.9955902,0.000059543923,0.0031713617,0.000061044855,0.000013870298,0.000011360483,0.00057013944,0.00001762917,0.0005048692],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998691,0.0000061053556,0.0000123102545,0.000031388066,0.000044538618,0.000036529327],"domain_scores_gemma":[0.9996507,0.00004486842,0.000081264036,0.000028914083,0.00003490832,0.00015930888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014053276,0.00027874918,0.00037542175,0.0009806425,0.0009791044,0.0007366394,0.0002859816,0.00051301654,0.0011218229],"category_scores_gemma":[0.000522028,0.00027110163,0.00017982213,0.0008578958,0.00036205657,0.00041391762,0.00093567773,0.0005016998,0.0003067167],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006963528,0.00032487346,0.8780704,0.00013352439,0.00009979013,0.008588938,0.0016771103,0.0011364021,0.06626068,0.001249627,0.0014686087,0.04029376],"study_design_scores_gemma":[0.00010556513,0.00039800216,0.9529743,0.00002353682,0.000092294,0.013744294,0.0008308331,0.0054326076,0.01657006,0.001034866,0.008755067,0.000038657945],"about_ca_topic_score_codex":0.0031435112,"about_ca_topic_score_gemma":0.00875887,"teacher_disagreement_score":0.0031435112,"about_ca_system_score_codex":0.00039404578,"about_ca_system_score_gemma":0.00024752604,"threshold_uncertainty_score":0.006250441},"labels":[],"label_agreement":null},{"id":"W2023378469","doi":"10.1086/380831","title":"An Interstellar Origin for the Beryllium 10 in Calcium‐rich, Aluminum‐rich Inclusions","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Formation and evolution of the Solar System; Astrophysics; Spallation; Cosmic ray; Nucleosynthesis; Supernova; Beryllium; Cosmic ray spallation; Solar System; Molecular cloud; Astronomy; Astrobiology; Neutron; Nuclear physics; Stars","score_opus":0.017223154079282557,"score_gpt":0.2697411167664698,"score_spread":0.25251796268718724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023378469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99176276,0.00017905554,0.0039732596,0.00009737551,0.000014595722,0.000017721039,0.00012142292,0.00004909206,0.0037847755],"genre_scores_gemma":[0.9981768,0.00007793917,0.0012428374,0.000016033438,0.0000038624967,0.0000056460613,0.00006717847,0.000017581266,0.00039218747],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99995244,0.0000048075303,0.0000023095665,0.000010190266,0.000012868515,0.000017378488],"domain_scores_gemma":[0.9998135,0.000059944614,0.000055564466,0.000011671374,0.000024303738,0.000035095403],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014472487,0.00039498942,0.00025495098,0.00026793816,0.000655812,0.00068147754,0.00068021356,0.0007270575,0.0011842602],"category_scores_gemma":[0.00078725023,0.00033283807,0.0004999895,0.0002706587,0.00052657543,0.00066010957,0.00042774944,0.0004189566,0.00017391157],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021458809,0.000121029145,0.12501787,0.00012906211,0.000112921996,0.0011991512,0.00018471731,0.8234556,0.035943568,0.008300465,0.00041605433,0.0049050287],"study_design_scores_gemma":[0.000092554845,0.00007288634,0.04074522,0.000030150752,0.000058410867,0.00022971952,0.00014448793,0.9456956,0.009952853,0.0018562333,0.0010927182,0.000029104463],"about_ca_topic_score_codex":0.026401162,"about_ca_topic_score_gemma":0.013694726,"teacher_disagreement_score":0.026401162,"about_ca_system_score_codex":0.0015708588,"about_ca_system_score_gemma":0.00088045275,"threshold_uncertainty_score":0.052495003},"labels":[],"label_agreement":null},{"id":"W2023489670","doi":"10.1088/0004-637x/700/2/1994","title":"ERRATUM: “QUIESCENT DENSE GAS IN PROTOSTELLAR CLUSTERS: THE OPHIUCHUS A CORE” (2004, APJ, 617, 425)","year":2009,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Physics; Core (optical fiber); Astrophysics; Astronomy; Stars; Molecular cloud; Optics","score_opus":0.00858387642693963,"score_gpt":0.24316213920799676,"score_spread":0.23457826278105712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023489670","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011271973,0.0012606252,0.00027060977,0.025173787,0.9645238,0.000025203226,0.001508107,0.00025675094,0.0058539743],"genre_scores_gemma":[0.03928401,0.013188427,0.004160668,0.091989845,0.3445088,0.00016761248,0.011336805,0.0019490655,0.49341473],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9991197,0.00007624335,0.00018861829,0.0001672017,0.00034826633,0.00009998859],"domain_scores_gemma":[0.99491066,0.0009446571,0.0004413636,0.0004019652,0.0028229482,0.00047846098],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010306608,0.0023986355,0.0014656481,0.003046498,0.004013075,0.0026105435,0.0023198063,0.0037031814,0.03742936],"category_scores_gemma":[0.011340507,0.0007776779,0.0011614176,0.0017805895,0.0015136725,0.001858319,0.0014385874,0.0042393785,0.023018995],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103406994,0.000016090782,0.00023717119,0.00011938916,0.000014633524,0.00050433545,0.00002294818,0.00006082498,0.00024891074,0.0004200924,0.99338067,0.004871506],"study_design_scores_gemma":[0.000069068206,0.0000806741,0.0067148195,0.00025999383,0.00008777584,0.0010344686,0.00020051145,0.00027241898,0.0013822049,0.0012175625,0.9886153,0.000065263186],"about_ca_topic_score_codex":0.018068617,"about_ca_topic_score_gemma":0.019245673,"teacher_disagreement_score":0.03742936,"about_ca_system_score_codex":0.0024894536,"about_ca_system_score_gemma":0.002749027,"threshold_uncertainty_score":0.12521368},"labels":[],"label_agreement":null},{"id":"W2023539392","doi":"10.1086/591661","title":"No Detectable Radio Emission from the Magnetar‐Like Pulsar in Kes 75","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Radio telescope; Green Bank Telescope; Supernova remnant; Millisecond pulsar; Telescope; Magnetic field; Supernova","score_opus":0.012051980811905208,"score_gpt":0.27073063565417727,"score_spread":0.25867865484227204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023539392","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99911934,0.0000636463,0.00006099646,0.000009204557,0.0000042709185,0.0000026677908,0.00010538761,0.000010040828,0.0006244274],"genre_scores_gemma":[0.99850595,0.00006139436,0.00018847223,0.000039994222,0.000010070085,0.0000052177693,0.0007179307,0.000006744514,0.0004641858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998957,0.000005328208,0.000009610579,0.000035076206,0.00002860157,0.000025664702],"domain_scores_gemma":[0.99973553,0.00002542814,0.00011693843,0.00002996867,0.000018565288,0.00007360452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013457841,0.00021910148,0.00032007118,0.0005681423,0.00048645475,0.0006833399,0.00027747484,0.00028886079,0.0014817726],"category_scores_gemma":[0.0003597073,0.00018960946,0.0001402507,0.00043154965,0.0003951003,0.00021450453,0.00054567517,0.00023624818,0.00040314457],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003924052,0.0001336243,0.8499011,0.00008497348,0.000118125856,0.0019662492,0.00055629713,0.00019035161,0.13622425,0.00025133052,0.00058160385,0.009599647],"study_design_scores_gemma":[0.00001188346,0.000079299374,0.9950375,0.0000061724754,0.000020447422,0.00085439376,0.000114790746,0.00009936755,0.0023031943,0.0000334915,0.0014343712,0.000005018345],"about_ca_topic_score_codex":0.0018390811,"about_ca_topic_score_gemma":0.0052933143,"teacher_disagreement_score":0.0018390811,"about_ca_system_score_codex":0.0002514609,"about_ca_system_score_gemma":0.00017870955,"threshold_uncertainty_score":0.0049570203},"labels":[],"label_agreement":null},{"id":"W2023559740","doi":"10.1086/521543","title":"The Cold Dark Matter Halos of Local Group Dwarf Spheroidals","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":190,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Dark matter; Galaxy; Astronomy; Dark matter halo; Cold dark matter; Velocity dispersion; Local Group; Dark galaxy; RADIUS; Milky Way; Halo","score_opus":0.006759719297211954,"score_gpt":0.19625676700897213,"score_spread":0.18949704771176018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023559740","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994978,0.000028481576,0.000076339005,0.000005505195,2.498391e-7,7.9819614e-7,0.000021954454,0.0000032234677,0.00036568628],"genre_scores_gemma":[0.9997631,0.000018769553,0.000053550208,0.0000026939074,7.424945e-7,5.161432e-7,0.00004519967,0.0000016137592,0.00011377693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996305,0.0000046325335,0.0000015202527,0.000009548917,0.0000069194984,0.000014281338],"domain_scores_gemma":[0.99965155,0.000048458973,0.00011905949,0.00003887213,0.00002995738,0.00011220555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015809953,0.00012084123,0.00017149908,0.0004922232,0.00033914752,0.0005265614,0.00012267365,0.000089435096,0.0010190012],"category_scores_gemma":[0.00046613882,0.00007587704,0.00015758465,0.0003088394,0.0003515614,0.00023034918,0.0005048215,0.00011364565,0.00015185785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017200632,0.000026480584,0.95959723,0.000026554299,0.000055938963,0.0005084277,0.0012954888,0.0061233263,0.022087215,0.0021333625,0.00022009766,0.007753794],"study_design_scores_gemma":[0.000007025446,0.000053016112,0.99065673,0.000006979029,0.000012845301,0.00014429,0.0005806957,0.0058109094,0.0013688803,0.0007377136,0.000612813,0.000008080287],"about_ca_topic_score_codex":0.0072245607,"about_ca_topic_score_gemma":0.007305699,"teacher_disagreement_score":0.0072245607,"about_ca_system_score_codex":0.0003879666,"about_ca_system_score_gemma":0.00016797068,"threshold_uncertainty_score":0.014365017},"labels":[],"label_agreement":null},{"id":"W2023668546","doi":"10.1088/0004-637x/755/2/110","title":"RADIO AND X-RAY OBSERVATIONS OF SN 2006jd: ANOTHER STRONGLY INTERACTING TYPE IIn SUPERNOVA","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Giant Metrewave Radio Telescope; Physics; Astrophysics; Supernova; RADIUS; Line-of-sight; Line (geometry); Luminosity; Absorption (acoustics); Asymmetry; Emission spectrum; Wavelength; X-ray; Astronomy; Spectral line; Radio galaxy; Galaxy; Optics","score_opus":0.02724262456188444,"score_gpt":0.25256869772995183,"score_spread":0.22532607316806738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023668546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980038,0.0001721108,0.00036908832,0.000027008397,0.000024349609,0.000024014023,0.0005792023,0.000026626565,0.00077379285],"genre_scores_gemma":[0.98964477,0.00025707498,0.0029764764,0.00011429913,0.00007833296,0.000023680903,0.0055525233,0.000018194634,0.001334697],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959284,0.00003097781,0.000041402633,0.00011472961,0.00013868073,0.000081403756],"domain_scores_gemma":[0.9987759,0.00004769704,0.00031952836,0.00011772484,0.00017778513,0.0005612919],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074402045,0.0006170166,0.00054348,0.0012173385,0.00096438406,0.0006725867,0.00066717586,0.00060135574,0.00036891745],"category_scores_gemma":[0.00046511798,0.00023838166,0.00049300876,0.00059072534,0.0003248676,0.00039758117,0.00096544356,0.0006464565,0.0003195239],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006212227,0.00094017666,0.9227201,0.00009438056,0.00029990214,0.0035127245,0.00062842114,0.0005436797,0.053600483,0.00019421968,0.00107972,0.015764987],"study_design_scores_gemma":[0.000024584602,0.0008206952,0.98671836,0.000006727071,0.000059111386,0.0035909244,0.00020834232,0.00042671594,0.003510232,0.000044976132,0.004572095,0.0000171639],"about_ca_topic_score_codex":0.0035364612,"about_ca_topic_score_gemma":0.008218877,"teacher_disagreement_score":0.0035364612,"about_ca_system_score_codex":0.00031322174,"about_ca_system_score_gemma":0.00028390178,"threshold_uncertainty_score":0.0070317388},"labels":[],"label_agreement":null},{"id":"W2023684619","doi":"10.1086/521138","title":"The Gemini Deep Deep Survey. VIII. When Did Early‐Type Galaxies Form?","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Universe; Astronomy; Advanced Camera for Surveys; Stellar mass; Hubble Deep Field; Star formation","score_opus":0.009422601183642071,"score_gpt":0.2224329563559253,"score_spread":0.21301035517228323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023684619","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8560519,0.0034769382,0.0027037226,0.002308497,0.00016875181,0.000074426716,0.11639327,0.0004901686,0.018332219],"genre_scores_gemma":[0.9276366,0.0010085528,0.005144349,0.000500215,0.00015916223,0.000044788187,0.055435024,0.00011900301,0.009952276],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.000014050868,0.0000064127303,0.00003788839,0.000026587913,0.000032781758],"domain_scores_gemma":[0.9994955,0.000028482435,0.00016196743,0.00007910376,0.00007677764,0.00015824065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043959395,0.00027976677,0.00016448412,0.001030703,0.00026153072,0.00063989696,0.0003056492,0.0003394296,0.0018836699],"category_scores_gemma":[0.00083182857,0.00014216591,0.00014952668,0.0011518499,0.00015472471,0.00066534965,0.0004932019,0.000377565,0.0014997585],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035908836,0.00006719094,0.88625264,0.00015059624,0.0000644795,0.00017711033,0.0008431836,0.0002211636,0.007133644,0.0014205648,0.042943362,0.060366977],"study_design_scores_gemma":[0.000006370739,0.000015418227,0.9725292,0.000012644778,0.000013029913,0.000090626585,0.00016819955,0.00021994379,0.0009465318,0.0002907209,0.025701474,0.0000056820695],"about_ca_topic_score_codex":0.011381586,"about_ca_topic_score_gemma":0.026388528,"teacher_disagreement_score":0.011381586,"about_ca_system_score_codex":0.00070497516,"about_ca_system_score_gemma":0.00017399267,"threshold_uncertainty_score":0.022630692},"labels":[],"label_agreement":null},{"id":"W2023769663","doi":"10.1086/382204","title":"Water Absorption from Line‐of‐Sight Clouds toward W49A","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Line (geometry); Molecular cloud; Line-of-sight; Absorption (acoustics); Spectral line; Water vapor; Absorption spectroscopy; Satellite; Emission spectrum","score_opus":0.013541942006224186,"score_gpt":0.23374657872562124,"score_spread":0.22020463671939705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023769663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999148,0.000017328375,0.00009655798,0.000011440433,0.0000020594514,0.000004733142,0.00023805679,0.000013214705,0.0004686924],"genre_scores_gemma":[0.99888164,0.00002308972,0.00031654089,0.000016752343,0.000005189416,0.0000065400222,0.00055403064,0.00000563389,0.00019050438],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998722,0.000007573087,0.0000053649214,0.000039866412,0.00003369399,0.00004127746],"domain_scores_gemma":[0.9997614,0.00001780041,0.000071960945,0.000025955174,0.000040342493,0.00008256534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009807107,0.00018840093,0.0002483726,0.0005728812,0.000697548,0.00039016936,0.00042369266,0.00029457576,0.0013999162],"category_scores_gemma":[0.0002490413,0.00019189091,0.00021073894,0.0003853633,0.00020451276,0.00042170956,0.00048083437,0.0003385386,0.00031511558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022313824,0.00019092212,0.8658865,0.000023113997,0.00009010648,0.0002847508,0.0005686935,0.0005336983,0.124370515,0.00013925042,0.0005002856,0.007188966],"study_design_scores_gemma":[0.000020626678,0.00010217935,0.99346393,0.000007187258,0.000019917825,0.00009170704,0.00014253435,0.001602808,0.0037571301,0.00004594218,0.0007366553,0.000009234944],"about_ca_topic_score_codex":0.028413111,"about_ca_topic_score_gemma":0.06223162,"teacher_disagreement_score":0.028413111,"about_ca_system_score_codex":0.0003589417,"about_ca_system_score_gemma":0.00014459438,"threshold_uncertainty_score":0.056495488},"labels":[],"label_agreement":null},{"id":"W2023769689","doi":"10.1088/0004-637x/789/2/152","title":"FITTING FFT-DERIVED SPECTRA: THEORY, TOOL, AND APPLICATION TO SOLAR RADIO SPIKE DECOMPOSITION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Fast Fourier transform; Spectral line; Computer science; Algorithm; Distribution (mathematics); Frequency domain; Autoregressive model; Fourier transform; SIGNAL (programming language); Statistical physics; Spike (software development); Computational physics; Physics; Statistics; Mathematics; Mathematical analysis","score_opus":0.0029310352494909195,"score_gpt":0.21946874378860642,"score_spread":0.2165377085391155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2023769689","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0076055937,0.000038077043,0.9908957,0.00004433161,0.000011348344,0.000019874064,0.000045398396,0.0010118891,0.00032788783],"genre_scores_gemma":[0.12188845,0.0001997669,0.8763209,0.000031282492,0.000036910016,0.00007488809,0.00026768373,0.00064750534,0.00053265586],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9994986,0.00010431717,0.00004742479,0.000065450506,0.0002530073,0.000031286138],"domain_scores_gemma":[0.9979365,0.0011986434,0.00020664316,0.00023256325,0.00036844835,0.000057279885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019178687,0.0007856618,0.00044551535,0.0019418242,0.00059780694,0.0011529992,0.0010644109,0.00086155924,0.0017134382],"category_scores_gemma":[0.008127418,0.00040760924,0.0007101328,0.0015391968,0.0006124685,0.0014053342,0.0010402849,0.0010353591,0.00062382093],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011180032,0.00021378152,0.009995702,0.00025523873,0.000116232,0.00074261066,0.0007442495,0.3531073,0.0424966,0.058900505,0.003544903,0.5297711],"study_design_scores_gemma":[0.0000046458963,0.000016148038,0.0012671206,0.000014920144,0.0000052365494,0.00023528095,0.000055114033,0.9802735,0.005302874,0.011241644,0.0015648038,0.000018780598],"about_ca_topic_score_codex":0.0032569603,"about_ca_topic_score_gemma":0.0029045634,"teacher_disagreement_score":0.0032569603,"about_ca_system_score_codex":0.0005027278,"about_ca_system_score_gemma":0.0007685284,"threshold_uncertainty_score":0.010142803},"labels":[],"label_agreement":null},{"id":"W2024135564","doi":"10.1088/0004-637x/716/2/1136","title":"TESTING MASS LOSS IN LARGE MAGELLANIC CLOUD CEPHEIDS USING INFRARED AND OPTICAL OBSERVATIONS. II. PREDICTIONS AND TESTS OF THE OGLE-III FUNDAMENTAL-MODE CEPHEIDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cepheid variable; Astrophysics; Large Magellanic Cloud; Physics; Infrared; RADIUS; Wavelength; Effective radius; Luminosity; Astronomy; Galaxy; Stars; Optics","score_opus":0.01908467168724931,"score_gpt":0.2578488157205804,"score_spread":0.23876414403333107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024135564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987637,0.00004648076,0.0006885247,0.000034029697,0.0000015506623,0.0000045818983,0.00006682367,0.000011598655,0.00038278173],"genre_scores_gemma":[0.99955565,0.000011469028,0.00026975336,0.000013659547,0.0000029521211,0.0000028410775,0.00009934703,0.0000033749925,0.000040850835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999175,0.00029045896,0.000036346188,0.0002049036,0.00016414876,0.00012911885],"domain_scores_gemma":[0.99300176,0.0040980135,0.0014825999,0.0005331336,0.0002772698,0.00060717994],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017815917,0.0006384027,0.0003184598,0.0006732855,0.0006187768,0.0009523256,0.0009839615,0.00071685854,0.0012237442],"category_scores_gemma":[0.0078094206,0.00024524177,0.00050619425,0.0005646766,0.00092674326,0.0010070925,0.0009510996,0.000398556,0.00033794672],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043325895,0.0000693281,0.9849191,0.000016898462,0.00008403162,0.00013701762,0.000109717104,0.00800628,0.0030374434,0.00040140084,0.00007442247,0.0027111927],"study_design_scores_gemma":[0.00007607949,0.0004183901,0.9386433,0.000008938637,0.00006168524,0.00019497142,0.0005075394,0.056187477,0.0028693497,0.00076457165,0.00024997728,0.000017767483],"about_ca_topic_score_codex":0.009593138,"about_ca_topic_score_gemma":0.008571409,"teacher_disagreement_score":0.009593138,"about_ca_system_score_codex":0.00088747765,"about_ca_system_score_gemma":0.0003865932,"threshold_uncertainty_score":0.01907456},"labels":[],"label_agreement":null},{"id":"W2024177210","doi":"10.1086/588183","title":"A New Galaxy Group Finding Algorithm: Probability Friends‐of‐Friends","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Vision and Imaging","field":"Computer Science","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Redshift; Photometric redshift; Astrophysics; Galaxy; Algorithm; Galaxy group; Redshift survey; Astronomy; Velocity dispersion; Galaxy cluster; Computer science","score_opus":0.020563248726604588,"score_gpt":0.2607242798498761,"score_spread":0.24016103112327153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024177210","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.020213118,0.00027731044,0.97261435,0.00018273649,0.000105149215,0.00016184725,0.0004375347,0.003989546,0.002018327],"genre_scores_gemma":[0.15294784,0.0002036551,0.8397115,0.00012406035,0.0002065998,0.00026282368,0.0021578325,0.00043981892,0.003945908],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.997482,0.00034704403,0.000115005605,0.00082813,0.0010016585,0.00022620316],"domain_scores_gemma":[0.99563855,0.0014391536,0.0004666047,0.0012665234,0.0009204269,0.00026874314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002265072,0.0012409408,0.0019499933,0.006012378,0.0021768461,0.0026085975,0.004926399,0.0019277161,0.0049244496],"category_scores_gemma":[0.011504163,0.0008411642,0.0013637559,0.0036887832,0.0009365973,0.005543153,0.0032666882,0.0015084996,0.0036335],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004876796,0.00027942474,0.017193103,0.00021620293,0.00042846857,0.00029658552,0.0006043067,0.06648064,0.009096872,0.02566458,0.027175061,0.8520771],"study_design_scores_gemma":[0.000103260354,0.00009491358,0.0034753308,0.000026533035,0.00009471645,0.00065928214,0.00020593431,0.93244654,0.012237569,0.031179495,0.0193924,0.00008410865],"about_ca_topic_score_codex":0.0056850174,"about_ca_topic_score_gemma":0.006045459,"teacher_disagreement_score":0.006012378,"about_ca_system_score_codex":0.0010600146,"about_ca_system_score_gemma":0.0014627631,"threshold_uncertainty_score":0.01647389},"labels":[],"label_agreement":null},{"id":"W2024241823","doi":"10.1088/0004-637x/760/2/117","title":"EVOLUTIONARY TRACKS OF TRAPPED, ACCRETING PROTOPLANETS: THE ORIGIN OF THE OBSERVED MASS-PERIOD RELATION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Photoevaporation; Planet; Physics; Protoplanet; Exoplanet; Planetary migration; Astrophysics; Gas giant; Planetary mass; Astronomy; Accretion (finance); Protoplanetary disk","score_opus":0.023283756732872012,"score_gpt":0.24598234178089481,"score_spread":0.2226985850480228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024241823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955924,0.0001656461,0.0025936502,0.00005724374,0.0000018765417,0.0000037179846,0.00014842772,0.000026243159,0.0014107432],"genre_scores_gemma":[0.99750525,0.00009828506,0.0019466623,0.000006737813,0.0000035092794,0.0000042169136,0.00017117368,0.000007885028,0.00025630867],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995327,0.000008331348,0.000002300542,0.00002046173,0.000006641203,0.000008991658],"domain_scores_gemma":[0.9996779,0.000096521704,0.00012682978,0.000034496512,0.000022195862,0.00004218056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012621748,0.00010851297,0.00007881143,0.0005633099,0.00032490664,0.0006799929,0.00027185792,0.00036797067,0.00089549785],"category_scores_gemma":[0.0010157954,0.00015778372,0.00013850347,0.00036555252,0.000352984,0.00047049532,0.0003023605,0.00024790797,0.00017883534],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024183631,0.00006616212,0.85868096,0.000060836534,0.000056936566,0.0004490982,0.000978623,0.03512875,0.033361666,0.0323839,0.00076079805,0.03783053],"study_design_scores_gemma":[0.000022962611,0.00009780785,0.8343896,0.000028659962,0.00004816648,0.0012638154,0.00042714545,0.13222729,0.0045463676,0.02340025,0.0035139145,0.000034057048],"about_ca_topic_score_codex":0.001849578,"about_ca_topic_score_gemma":0.0018255512,"teacher_disagreement_score":0.001849578,"about_ca_system_score_codex":0.00048022787,"about_ca_system_score_gemma":0.00010158332,"threshold_uncertainty_score":0.0036776662},"labels":[],"label_agreement":null},{"id":"W2024245608","doi":"10.1088/0004-637x/721/1/670","title":"AN EXPLANATION OF REVERSED SPECTRAL-LINE BISECTORS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Photosphere; Flux (metallurgy); Line (geometry); Granulation; Boundary (topology); Stars; Convection; Spectral line; Mechanics; Geometry; Astronomy; Classical mechanics; Mathematical analysis","score_opus":0.01067163676010206,"score_gpt":0.239270617673454,"score_spread":0.22859898091335196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024245608","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75094754,0.0006496327,0.16697174,0.0014041115,0.00024808585,0.00009704089,0.0012589478,0.003089508,0.07533341],"genre_scores_gemma":[0.98715276,0.0000702538,0.010760642,0.00011692915,0.000028421859,0.000013001807,0.0002500877,0.00019701078,0.0014108539],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99958426,0.00006743648,0.000024704565,0.00013337343,0.00009989113,0.00009045185],"domain_scores_gemma":[0.9980989,0.00032422578,0.00035670618,0.00057152647,0.00048415767,0.00016453027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005896262,0.00028496995,0.00019540342,0.0014300859,0.0006283012,0.0011958098,0.0010624689,0.00064694736,0.0065172333],"category_scores_gemma":[0.0047906977,0.00019975465,0.00026754098,0.0012231983,0.0014231713,0.0015961409,0.0008746581,0.0008956463,0.0012358909],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011863433,0.000111526846,0.17028967,0.00023212812,0.000044450655,0.002495941,0.0021885505,0.009852977,0.06156638,0.57553506,0.009674339,0.16682267],"study_design_scores_gemma":[0.00017600077,0.00030694788,0.22845642,0.000106342406,0.00004989167,0.011259904,0.0018085409,0.08104959,0.04055407,0.57015264,0.06586412,0.0002155724],"about_ca_topic_score_codex":0.0016482162,"about_ca_topic_score_gemma":0.00073128275,"teacher_disagreement_score":0.0065172333,"about_ca_system_score_codex":0.00044061005,"about_ca_system_score_gemma":0.00030176612,"threshold_uncertainty_score":0.021802306},"labels":[],"label_agreement":null},{"id":"W2024279864","doi":"10.1088/0004-637x/782/1/19","title":"THE SCUBA-2 COSMOLOGY LEGACY SURVEY: ULTRALUMINOUS STAR-FORMING GALAXIES IN A<i>z</i>= 1.6 CLUSTER","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia; Dalhousie University","funders":"Key Programme; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Council; Leverhulme Trust; Deutsche Forschungsgemeinschaft; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Luminous infrared galaxy; Star formation; Galaxy cluster; Astronomy; Cluster (spacecraft); Active galactic nucleus; Submillimeter Array; Computer science","score_opus":0.00922284412463852,"score_gpt":0.21940137030847764,"score_spread":0.21017852618383912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024279864","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99885535,0.000023815815,0.0000571943,0.0000083213445,8.9010723e-7,0.0000048271568,0.0007553627,0.000010723323,0.0002835935],"genre_scores_gemma":[0.991619,0.000047833986,0.00054532016,0.000015654803,0.000011540795,0.000011784207,0.0073592914,0.000009620374,0.0003799163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998934,0.0000067367814,0.00000498485,0.000028954191,0.000026941858,0.000038894515],"domain_scores_gemma":[0.9995658,0.000023716191,0.00013866561,0.00005522579,0.000047048834,0.00016954122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013287357,0.00026919745,0.00021468765,0.00182032,0.0003351526,0.00047031126,0.00041447865,0.00016609929,0.0007885683],"category_scores_gemma":[0.0003680891,0.0001233835,0.00021949163,0.0011384164,0.00020315559,0.00021653125,0.00061171013,0.00021802347,0.00038989517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000105167346,0.00007731382,0.9833576,0.000017708968,0.000047141886,0.00019715457,0.00024288017,0.0008320926,0.010111729,0.00018194907,0.001047573,0.0037817415],"study_design_scores_gemma":[0.000005329974,0.000009660922,0.9984059,0.0000017702099,0.000006440971,0.000044765216,0.0000504442,0.0008442148,0.00026125406,0.000017616909,0.00035015112,0.0000024110352],"about_ca_topic_score_codex":0.023110678,"about_ca_topic_score_gemma":0.040660642,"teacher_disagreement_score":0.023110678,"about_ca_system_score_codex":0.00028657526,"about_ca_system_score_gemma":0.00026220208,"threshold_uncertainty_score":0.04595232},"labels":[],"label_agreement":null},{"id":"W2024303055","doi":"10.1088/0004-637x/750/1/30","title":"A HYBRID SCENARIO FOR THE FORMATION OF BROWN DWARFS AND VERY LOW MASS STARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Brown dwarf; Stars; Low Mass; Stellar mass; Stellar evolution","score_opus":0.012006824230291972,"score_gpt":0.23004499527981528,"score_spread":0.2180381710495233,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024303055","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9323231,0.00026384028,0.053560793,0.00028528727,0.000025385434,0.000039037288,0.00018966351,0.00015232568,0.013160468],"genre_scores_gemma":[0.9924839,0.00006778402,0.005369857,0.000049955594,0.000009247203,0.000022892045,0.000079528356,0.000015453059,0.0019013736],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986947,0.00003923057,0.0000060932593,0.00003372939,0.000024511872,0.000026968923],"domain_scores_gemma":[0.9997702,0.0000673688,0.00003803213,0.000029875626,0.000019660034,0.000074859316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003272166,0.00037665296,0.00038583935,0.00042043292,0.000518139,0.0010969307,0.0011785463,0.0010454367,0.002551501],"category_scores_gemma":[0.0008613536,0.0002265162,0.00069201033,0.00029377447,0.0005431797,0.0011228593,0.0009864748,0.0004119066,0.00044314348],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045232,0.00026835364,0.14877042,0.00018573651,0.0003281644,0.005837941,0.00075236306,0.5785091,0.022002647,0.22077687,0.0016266945,0.020489361],"study_design_scores_gemma":[0.0001756939,0.00028312148,0.020076998,0.000018582501,0.00010490802,0.0023672027,0.0005036956,0.89506966,0.0035348576,0.07333111,0.004477354,0.00005689277],"about_ca_topic_score_codex":0.0016258268,"about_ca_topic_score_gemma":0.0013297512,"teacher_disagreement_score":0.002551501,"about_ca_system_score_codex":0.00037452078,"about_ca_system_score_gemma":0.00026151974,"threshold_uncertainty_score":0.008535624},"labels":[],"label_agreement":null},{"id":"W2024332245","doi":"10.1088/0004-637x/775/2/88","title":"LOW-VELOCITY SHOCKS TRACED BY EXTENDED SiO EMISSION ALONG THE W43 RIDGES: WITNESSING THE FORMATION OF YOUNG MASSIVE CLUSTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Velocity dispersion; Molecular cloud; Stars; Shock wave; Luminosity; Star formation; Shock (circulatory); Dispersion (optics)","score_opus":0.008024289043834837,"score_gpt":0.22855163805306303,"score_spread":0.22052734900922819,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024332245","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99973375,0.000014503172,0.000080641024,0.000003269935,3.109326e-7,0.0000012781336,0.000022387481,0.000005115729,0.00013874724],"genre_scores_gemma":[0.99966145,0.000017175656,0.0002052375,0.0000033902477,0.0000013899969,0.0000015860599,0.00005740462,0.000002536129,0.000049844424],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996114,0.0000030445374,0.0000018660593,0.000010671957,0.000008852933,0.000014470133],"domain_scores_gemma":[0.9998166,0.00002142647,0.00007811167,0.000018912726,0.000015901524,0.000049197926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010033718,0.000104985746,0.00010721085,0.00032053867,0.0002164233,0.00026726665,0.0002064148,0.00021355721,0.00036201035],"category_scores_gemma":[0.00029485844,0.00013478196,0.00011082444,0.0003026847,0.00020103484,0.00013098757,0.00040243397,0.00021572737,0.00010069421],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012315591,0.000036066023,0.9031048,0.000020099858,0.00003128711,0.0006972545,0.0006573307,0.0006858343,0.089331575,0.00026090263,0.000119196746,0.004932416],"study_design_scores_gemma":[0.0000025874451,0.00003263681,0.995861,0.0000023637292,0.0000073394776,0.00017363035,0.00014006945,0.0013852791,0.0021435223,0.00005942781,0.00018919793,0.0000029114406],"about_ca_topic_score_codex":0.0026086695,"about_ca_topic_score_gemma":0.0052626245,"teacher_disagreement_score":0.0026086695,"about_ca_system_score_codex":0.000117627096,"about_ca_system_score_gemma":0.00007835087,"threshold_uncertainty_score":0.005186975},"labels":[],"label_agreement":null},{"id":"W2024349663","doi":"10.1086/340118","title":"A Measurement by BOOMERANG of Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":817,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Spectral density; Microwave; COSMIC cancer database; Angular spectrum method; Spectrum (functional analysis); Cosmic infrared background; Background radiation","score_opus":0.013586188287964965,"score_gpt":0.21784084989644967,"score_spread":0.2042546616084847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024349663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9803398,0.00051556516,0.012388518,0.000116475734,0.000020580335,0.000010919518,0.0004250903,0.00031306938,0.005869922],"genre_scores_gemma":[0.99746895,0.000078415964,0.0017648945,0.00003000313,0.000014030744,0.0000057653765,0.0002343378,0.000033622233,0.00037002188],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99977964,0.0000321429,0.0000037306957,0.00007628601,0.000056776214,0.000051568735],"domain_scores_gemma":[0.99960035,0.00010158956,0.000095271964,0.00007466908,0.000041623185,0.00008653987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002482727,0.0003755465,0.0002522127,0.0009431298,0.00039338222,0.00051464944,0.00024785785,0.00024891124,0.0012509034],"category_scores_gemma":[0.0007430522,0.00026610796,0.00015890737,0.00055587984,0.0003882913,0.0005078662,0.0006335238,0.00058372086,0.00022833244],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026842186,0.00015225554,0.34986243,0.00014470927,0.00046962727,0.00047354266,0.0007791645,0.0016489187,0.5276264,0.008998949,0.0012959605,0.105863824],"study_design_scores_gemma":[0.00007590233,0.0002176513,0.9005327,0.000018679222,0.00016614729,0.0009041024,0.00011335546,0.0036198823,0.08211645,0.003534403,0.008626924,0.00007381613],"about_ca_topic_score_codex":0.0010761634,"about_ca_topic_score_gemma":0.003666775,"teacher_disagreement_score":0.0012509034,"about_ca_system_score_codex":0.00023842893,"about_ca_system_score_gemma":0.00011495651,"threshold_uncertainty_score":0.0041846633},"labels":[],"label_agreement":null},{"id":"W2024381971","doi":"10.1088/0004-637x/747/1/37","title":"A QUANTUM BAND MODEL OF THE ν<sub>3</sub>FUNDAMENTAL OF METHANOL (CH<sub>3</sub>OH) AND ITS APPLICATION TO FLUORESCENCE SPECTRA OF COMETS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of New Brunswick","funders":"","keywords":"Physics; Spectral line; Emission spectrum; Infrared; Spectroscopy; Fluorescence; Wavelength; Spectral resolution; Infrared spectroscopy; Astrophysics; Astronomy; Optics","score_opus":0.012095880541412462,"score_gpt":0.2216065362589444,"score_spread":0.2095106557175319,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024381971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.73641396,0.00040058652,0.24129698,0.0010201726,0.00014463344,0.00011123218,0.00045413943,0.0002570393,0.01990122],"genre_scores_gemma":[0.9773292,0.00018632588,0.019095609,0.00015685557,0.00004973661,0.00013840766,0.00018192685,0.00011230937,0.002749556],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993014,0.000017879573,0.0000027384744,0.00001250688,0.00001921479,0.000017537695],"domain_scores_gemma":[0.99978215,0.000083380815,0.00003173177,0.000027791233,0.000039857805,0.000035180026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000292235,0.0003384736,0.0004041144,0.00022803308,0.00085635995,0.000563075,0.001105337,0.0010933403,0.0020406186],"category_scores_gemma":[0.0005810484,0.00029846877,0.00078792946,0.00026491616,0.0011270472,0.0009765835,0.0003651057,0.0005633005,0.00029577376],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000361075,0.000056838886,0.0010636066,0.00002103787,0.000015212507,0.00009489129,0.00007099002,0.96149594,0.00621077,0.028922208,0.00051403773,0.0014983559],"study_design_scores_gemma":[0.000015676105,0.000011218881,0.00029320203,0.0000013803533,0.0000041267235,0.00000854072,0.000010040976,0.99640226,0.00031097757,0.0026717118,0.00026573712,0.0000051148704],"about_ca_topic_score_codex":0.013708174,"about_ca_topic_score_gemma":0.006435434,"teacher_disagreement_score":0.013708174,"about_ca_system_score_codex":0.0012594602,"about_ca_system_score_gemma":0.00070099736,"threshold_uncertainty_score":0.027256787},"labels":[],"label_agreement":null},{"id":"W2024454353","doi":"10.1086/512362","title":"High‐Resolution Imaging of Warm and Dense Molecular Gas in the Nuclear Region of the Luminous Infrared Galaxy NGC 6240","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Outflow; Galaxy; Infrared; Luminous infrared galaxy; Submillimeter Array; Velocity gradient; Star formation; Astronomy","score_opus":0.004674875335602471,"score_gpt":0.19248032593169812,"score_spread":0.18780545059609566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024454353","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957982,0.00018563034,0.00048454182,0.00003687641,0.0000028918012,0.0000033555145,0.00025774186,0.00013102569,0.00309987],"genre_scores_gemma":[0.9967367,0.0001416239,0.001586496,0.0000467894,0.000009043047,0.000008406111,0.00046891833,0.000013765625,0.0009882416],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993813,0.0000031160434,0.0000019600345,0.000015348767,0.00001811504,0.000023427878],"domain_scores_gemma":[0.9999168,0.0000104374,0.000022424147,0.0000068850227,0.000011998741,0.00003143324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010924086,0.00014141109,0.00013022638,0.0008832659,0.00022628892,0.00027186648,0.0001964123,0.00022617543,0.0018525319],"category_scores_gemma":[0.00016903931,0.0001842,0.00012935647,0.0003736567,0.00012809965,0.00014466043,0.00032874063,0.00012885824,0.00030684893],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023685764,0.00006768272,0.1138684,0.00009497613,0.0000499816,0.0008784422,0.0004677019,0.0011591512,0.8535541,0.00032485058,0.0013347736,0.02796302],"study_design_scores_gemma":[0.000021221922,0.00010427522,0.9809776,0.000020656864,0.0000320158,0.0007438223,0.00016710749,0.0021065813,0.012539332,0.00019499393,0.003079094,0.00001327273],"about_ca_topic_score_codex":0.006112636,"about_ca_topic_score_gemma":0.013537567,"teacher_disagreement_score":0.006112636,"about_ca_system_score_codex":0.0002754206,"about_ca_system_score_gemma":0.00010032885,"threshold_uncertainty_score":0.012154102},"labels":[],"label_agreement":null},{"id":"W2024520165","doi":"10.1086/511669","title":"Near‐Infrared Properties of Moderate‐Redshift Galaxy Clusters: Luminosity Functions and Density Profiles","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"York University; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Redshift; Luminosity; Luminosity function; Galaxy; Cluster (spacecraft); Galaxy cluster; Astronomy; Stars","score_opus":0.011488360446638346,"score_gpt":0.20245453604238883,"score_spread":0.1909661755957505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024520165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99752766,0.00007676237,0.00021311923,0.000014232364,7.671457e-7,0.000004438656,0.0009829631,0.00004772028,0.001132394],"genre_scores_gemma":[0.99827516,0.00002722529,0.00023217141,0.0000048486645,0.000001641092,0.0000028902714,0.0011959512,0.0000069044463,0.00025314602],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999101,0.0000029470236,0.0000025983345,0.000017942037,0.000023940667,0.00004239008],"domain_scores_gemma":[0.9995297,0.000059333335,0.000098032404,0.000036494577,0.00009474751,0.00018163535],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014022143,0.00019674838,0.00016818191,0.0015902921,0.00042774618,0.0004459658,0.00034883496,0.0001795778,0.0018150181],"category_scores_gemma":[0.00041581274,0.00012530334,0.00023255018,0.0009885263,0.00027426032,0.00015167987,0.00029561168,0.00012819716,0.00027517127],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019352268,0.000048844176,0.96911937,0.00003304767,0.000060696155,0.00010736413,0.000429936,0.004167969,0.010187218,0.0005721853,0.001417596,0.013662277],"study_design_scores_gemma":[0.0000014760295,0.00000960408,0.99765223,0.0000017502542,0.0000057347156,0.00003580542,0.000051238734,0.0016424386,0.0002823395,0.000045485664,0.00026697406,0.0000048980287],"about_ca_topic_score_codex":0.15194346,"about_ca_topic_score_gemma":0.15717521,"teacher_disagreement_score":0.15194346,"about_ca_system_score_codex":0.0008229245,"about_ca_system_score_gemma":0.00037219375,"threshold_uncertainty_score":0.30211806},"labels":[],"label_agreement":null},{"id":"W2024551212","doi":"10.1088/0004-637x/698/2/1893","title":"GEOMETRICAL PROPERTIES OF AVALANCHES IN A PSEUDO-3D CORONAL LOOP","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec; Université de Montréal","funders":"","keywords":"Physics; Fractal; Coronal loop; Fractal dimension; Solar flare; Superposition principle; Computational physics; Statistical physics; Geometry; Astrophysics; Mechanics; Magnetic field; Mathematical analysis; Solar wind; Coronal mass ejection","score_opus":0.011811102692290208,"score_gpt":0.21959443921487848,"score_spread":0.20778333652258826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024551212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955649,0.000022691644,0.0040180054,0.000014376444,0.0000023243288,0.000003875136,0.000028796727,0.000034861194,0.0003100975],"genre_scores_gemma":[0.99871004,0.000009210883,0.0011498609,0.000003158081,0.000001000814,0.0000035653165,0.000051417217,0.0000067651304,0.000064982756],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999198,0.000016051084,0.0000049693886,0.000017289447,0.000022584101,0.000019388874],"domain_scores_gemma":[0.9993795,0.00023608824,0.00014254103,0.00006467091,0.000078737256,0.00009848485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021001663,0.00018284944,0.00018046162,0.0005565796,0.00025966155,0.00044008472,0.00032305036,0.0003082402,0.00060604425],"category_scores_gemma":[0.0012248019,0.00013826106,0.00032958257,0.00023044016,0.0004913906,0.0003407222,0.00026578846,0.00021297242,0.000043567612],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030838395,0.00010629728,0.026420858,0.000056669338,0.00008553723,0.0005641897,0.00034227094,0.89267236,0.06406018,0.009930772,0.00026891506,0.00518357],"study_design_scores_gemma":[0.00001794164,0.00010747074,0.007061775,0.0000030931312,0.000007870307,0.00011397958,0.000061571525,0.9855584,0.0046860557,0.0021733602,0.0001956666,0.0000129356395],"about_ca_topic_score_codex":0.0011693019,"about_ca_topic_score_gemma":0.00055126986,"teacher_disagreement_score":0.0011693019,"about_ca_system_score_codex":0.0004270422,"about_ca_system_score_gemma":0.0001553367,"threshold_uncertainty_score":0.0030983686},"labels":[],"label_agreement":null},{"id":"W2024655466","doi":"10.1088/0004-637x/698/1/83","title":"INDIVIDUAL AND GROUP GALAXIES IN CNOC1 CLUSTERS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Brightest cluster galaxy; Galaxy group; Astronomy; Galaxy cluster; Interacting galaxy; Lenticular galaxy; Galaxy formation and evolution; Galaxy","score_opus":0.00756668606200127,"score_gpt":0.20936883556714753,"score_spread":0.20180214950514624,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024655466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989722,0.00006204,0.000035736488,0.000009021135,6.132324e-7,0.0000029265475,0.00051009556,0.0000072499156,0.00040021783],"genre_scores_gemma":[0.99782974,0.000041480842,0.000111891524,0.00000632834,0.0000015482552,0.0000030441443,0.0016950641,0.0000066942407,0.00030413267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99943095,0.000023338278,0.000012601973,0.00022348974,0.00016141067,0.00014814078],"domain_scores_gemma":[0.9986771,0.00018930188,0.0003309705,0.00016280556,0.00026042468,0.00037946767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045860087,0.00022596269,0.00044916556,0.0028032667,0.0008837707,0.0009352005,0.00062237255,0.0002782752,0.0012052066],"category_scores_gemma":[0.0023113338,0.00021061237,0.0001778867,0.0020978805,0.0006128492,0.00029220962,0.0009131483,0.00019500288,0.00017241268],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001626073,0.000021707787,0.989042,0.000018544702,0.000053185224,0.00004931915,0.00065996544,0.0008959977,0.002135206,0.00024213218,0.00043600737,0.00628331],"study_design_scores_gemma":[0.0000019665279,0.0000043779582,0.9990441,0.0000020686598,0.000006659724,0.000016084296,0.00012338087,0.00048563976,0.00012026957,0.000022897815,0.00016879934,0.0000037305401],"about_ca_topic_score_codex":0.38210633,"about_ca_topic_score_gemma":0.51526827,"teacher_disagreement_score":0.38210633,"about_ca_system_score_codex":0.0027098646,"about_ca_system_score_gemma":0.0008353764,"threshold_uncertainty_score":0.75976443},"labels":[],"label_agreement":null},{"id":"W2024682279","doi":"10.1086/379648","title":"Morphological Analysis of H<scp>i</scp>Features. I. Metric Space Technique","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Université Laval","funders":"","keywords":"Physics; Fractal dimension; Galactic plane; Formalism (music); Astrophysics; Pixel; Fractal; Metric (unit); Galaxy; Mathematical analysis; Mathematics; Optics","score_opus":0.006830371577544607,"score_gpt":0.2197823138140403,"score_spread":0.2129519422364957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024682279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5595687,0.002796844,0.39024055,0.00050661835,0.00016050106,0.0003002426,0.0023606308,0.0010290879,0.043036852],"genre_scores_gemma":[0.84824777,0.0011142569,0.14515787,0.00006559164,0.00008771492,0.00007379295,0.0014709334,0.00012568296,0.003656411],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99975747,0.000022834452,0.00001626456,0.000037851445,0.00013351056,0.000032200667],"domain_scores_gemma":[0.9995339,0.00006631442,0.00012948627,0.00006660419,0.0001655005,0.00003813517],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026201815,0.00025870744,0.00018888117,0.0031582473,0.0004242138,0.0013058946,0.00038843125,0.00020717808,0.0016142519],"category_scores_gemma":[0.0009865735,0.00011624367,0.00046996083,0.002806378,0.00070361194,0.00081841537,0.00051243295,0.00029809342,0.00044067157],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027833262,0.0000573844,0.14331716,0.0006286635,0.0002413735,0.0012381427,0.0010817874,0.012678034,0.22778566,0.054655127,0.0064251735,0.5516132],"study_design_scores_gemma":[0.000022034752,0.00030567189,0.8041376,0.00008840891,0.00009275782,0.004240223,0.0013710177,0.0518597,0.059573434,0.022268541,0.05591253,0.0001280936],"about_ca_topic_score_codex":0.0053156884,"about_ca_topic_score_gemma":0.0045710863,"teacher_disagreement_score":0.0053156884,"about_ca_system_score_codex":0.0005852414,"about_ca_system_score_gemma":0.00032416687,"threshold_uncertainty_score":0.010569513},"labels":[],"label_agreement":null},{"id":"W2024760743","doi":"10.1086/323959","title":"Discovery and Asteroseismological Analysis of the Pulsating sdB Star PG 0014+067","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Amplitude; Subdwarf; Light curve; Asteroseismology; Stars; Oscillation (cell signaling); Telescope; Instability strip; Luminosity; Rotation period; Astronomy; White dwarf; Cepheid variable; Optics","score_opus":0.012861376893692988,"score_gpt":0.22752301042338338,"score_spread":0.2146616335296904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024760743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99905604,0.000046666144,0.00024420902,0.000017117569,0.0000025953948,0.0000055962555,0.0000945245,0.000008487035,0.00052473234],"genre_scores_gemma":[0.998331,0.000056760597,0.00080393784,0.000010163443,0.000005446048,0.0000068083327,0.0005400949,0.0000035787998,0.00024220151],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999558,0.0000036128972,0.000002589414,0.000012355618,0.00001686344,0.000008816497],"domain_scores_gemma":[0.9998605,0.000013735295,0.000038628496,0.00001491194,0.000017247909,0.00005496267],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009788439,0.00018145893,0.00025054577,0.00062572316,0.00036732157,0.0004247961,0.00025846635,0.00028398135,0.0008020239],"category_scores_gemma":[0.00023046386,0.0001108625,0.00017824293,0.000530937,0.00029014423,0.00010914829,0.00046880174,0.00024002808,0.00025614217],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029153412,0.00013667956,0.8250506,0.00009080568,0.00007545312,0.0016542717,0.0004105624,0.0013905788,0.14152977,0.00063759484,0.0003027137,0.028429477],"study_design_scores_gemma":[0.0000148543295,0.00032259058,0.98380834,0.000008321399,0.00003049969,0.0010677812,0.00021579978,0.003244077,0.008082759,0.00034144794,0.00285104,0.000012428266],"about_ca_topic_score_codex":0.0012396661,"about_ca_topic_score_gemma":0.0020045568,"teacher_disagreement_score":0.0012396661,"about_ca_system_score_codex":0.000243994,"about_ca_system_score_gemma":0.00018852564,"threshold_uncertainty_score":0.0026829839},"labels":[],"label_agreement":null},{"id":"W2024843589","doi":"10.1088/0004-637x/751/1/50","title":"THE DEEP2 GALAXY REDSHIFT SURVEY: THE VORONOI-DELAUNAY METHOD CATALOG OF GALAXY GROUPS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Victoria","funders":"","keywords":"Galaxy; Redshift; Cosmology; Galaxy group; Galaxy formation and evolution; Redshift survey; Galaxy cluster; Interacting galaxy","score_opus":0.012907751387179504,"score_gpt":0.24754712615983326,"score_spread":0.23463937477265376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024843589","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.644772,0.00055492134,0.12718737,0.00031407914,0.000057096335,0.0007123045,0.20235954,0.0072825043,0.01676017],"genre_scores_gemma":[0.4796448,0.00016641311,0.12579565,0.00008265322,0.00004107516,0.0006054232,0.38934082,0.0007406186,0.0035824855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989874,0.00019795023,0.000049493276,0.00023986315,0.00042305893,0.000102242004],"domain_scores_gemma":[0.9979448,0.000246122,0.00024159026,0.00093308615,0.00046824137,0.00016614566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001099892,0.00051466265,0.000537523,0.00403252,0.0005039222,0.0009666484,0.0015262368,0.00033568023,0.006309029],"category_scores_gemma":[0.005337218,0.00041518992,0.00041718732,0.00417433,0.0003309847,0.0008714873,0.001817227,0.0004007946,0.002713851],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010358588,0.0004701729,0.41736,0.000555526,0.00035613796,0.0003248588,0.0010850377,0.11559608,0.017199125,0.021770798,0.15514456,0.26910186],"study_design_scores_gemma":[0.00092307123,0.0002701193,0.3900184,0.00011118485,0.00011130102,0.0007415816,0.00063580036,0.3199279,0.022075554,0.019191172,0.24580175,0.00019218898],"about_ca_topic_score_codex":0.016949425,"about_ca_topic_score_gemma":0.020792771,"teacher_disagreement_score":0.016949425,"about_ca_system_score_codex":0.000902906,"about_ca_system_score_gemma":0.0011137393,"threshold_uncertainty_score":0.03370154},"labels":[],"label_agreement":null},{"id":"W2024869979","doi":"10.1086/510199","title":"Are High‐Redshift Quasars Blurry?","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Redshift; Cosmology; Hubble space telescope; Observational cosmology; Galaxy; Planck; Hubble's law; Plane (geometry)","score_opus":0.00854693912721211,"score_gpt":0.2536547189952725,"score_spread":0.24510777986806037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024869979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9691761,0.01552888,0.0023270317,0.0054344153,0.000118038886,0.000019849089,0.00017732414,0.00008440462,0.0071338797],"genre_scores_gemma":[0.99727017,0.0014534319,0.00022374128,0.0003957342,0.00014227409,0.0000017419654,0.000049830815,0.0000054048164,0.00045758433],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987947,0.0001853985,0.000091548834,0.0002642886,0.00036052108,0.0003035527],"domain_scores_gemma":[0.9891278,0.0018864658,0.005899264,0.00127412,0.0010071691,0.00080510735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019510884,0.0003262152,0.0006214882,0.0022674762,0.000994684,0.0026863255,0.0007279062,0.0018724238,0.005208765],"category_scores_gemma":[0.018387532,0.00045208915,0.0003108321,0.0017803032,0.0028418205,0.0032290677,0.0010617165,0.00082063326,0.00084270776],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004735517,0.00011566026,0.8208225,0.00035670964,0.00021779817,0.0041904715,0.008072482,0.0001977481,0.0066887247,0.015240292,0.0038387903,0.13978519],"study_design_scores_gemma":[0.00001809951,0.00010866782,0.9682406,0.000078079705,0.000089398956,0.008026908,0.0030051726,0.0003241519,0.0014151986,0.0116685275,0.006995533,0.000029664243],"about_ca_topic_score_codex":0.004555521,"about_ca_topic_score_gemma":0.003243627,"teacher_disagreement_score":0.005208765,"about_ca_system_score_codex":0.0008746993,"about_ca_system_score_gemma":0.00029446656,"threshold_uncertainty_score":0.01742506},"labels":[],"label_agreement":null},{"id":"W2024904309","doi":"10.1086/588599","title":"IRAC Excess in Distant Star‐Forming Galaxies: Tentative Evidence for the 3.3 μm Polycyclic Aromatic Hydrocarbon Feature?","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Galaxy; Luminous infrared galaxy; James Webb Space Telescope; Spectral energy distribution; Astrophysics; Physics; Feature (linguistics); Spitzer Space Telescope; Polycyclic aromatic hydrocarbon; Star (game theory); Astronomy; Star formation; Telescope; Astrobiology","score_opus":0.023803740799172517,"score_gpt":0.2629923848593842,"score_spread":0.23918864406021167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024904309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989581,0.00016749959,0.00018471843,0.000019479896,0.000002268386,0.0000023770372,0.00008984797,0.000020964173,0.0005547152],"genre_scores_gemma":[0.9996482,0.00003681935,0.00013532669,0.000013235817,0.000004275637,8.731766e-7,0.00009784395,0.0000021522412,0.000061275256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983597,0.000011311524,0.00000985078,0.00005599111,0.000041185056,0.000045582394],"domain_scores_gemma":[0.9992568,0.00008889293,0.0002850029,0.000104567305,0.000056681238,0.00020797715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000247334,0.00019778777,0.00026088173,0.0009273019,0.00022843371,0.0005108516,0.00031060193,0.0003863331,0.0017346605],"category_scores_gemma":[0.00046921484,0.00013666823,0.00022276762,0.0004989892,0.00039885155,0.00020043232,0.00030059458,0.00018281944,0.00057982386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009402563,0.000036015717,0.9523875,0.00002162181,0.000033083812,0.000333373,0.000092916904,0.00009309501,0.041526917,0.000093636554,0.000066566594,0.005221335],"study_design_scores_gemma":[0.000001966659,0.000033104585,0.99811745,0.0000018505029,0.000010754518,0.00034836467,0.000029325709,0.0001273167,0.0011323527,0.000038951493,0.00015699083,0.0000016343421],"about_ca_topic_score_codex":0.001539213,"about_ca_topic_score_gemma":0.0024663308,"teacher_disagreement_score":0.0017346605,"about_ca_system_score_codex":0.00020653056,"about_ca_system_score_gemma":0.00008197582,"threshold_uncertainty_score":0.0058030486},"labels":[],"label_agreement":null},{"id":"W2024993898","doi":"10.1088/0004-637x/799/1/97","title":"THE STAR-FORMING HISTORIES OF THE NUCLEUS, BULGE, AND INNER DISK OF NGC 5102: CLUES TO THE EVOLUTION OF A NEARBY LENTICULAR GALAXY<sup>,</sup><sup>,</sup>","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Bulge; Physics; Astrophysics; Galaxy; Astronomy; Luminosity; Stars; Star formation","score_opus":0.009438776229039273,"score_gpt":0.21096129180635947,"score_spread":0.2015225155773202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2024993898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983961,0.00003848282,0.000076638935,0.000015311014,7.978974e-7,0.0000020805498,0.0005671717,0.000011657696,0.0008917584],"genre_scores_gemma":[0.9981007,0.000038391423,0.00029961538,0.000011711915,0.0000024153744,0.0000022314416,0.0011637637,0.0000046502805,0.0003765409],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996924,0.0000019217878,0.0000024087155,0.0000116698075,0.0000067339197,0.000008078985],"domain_scores_gemma":[0.99988925,0.000009012064,0.00002953001,0.000011271679,0.00001616766,0.000044633787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000091042646,0.0001277649,0.000069012036,0.0005318824,0.00025268664,0.00031243736,0.00017358238,0.0001906044,0.0015035169],"category_scores_gemma":[0.00014801505,0.00012834407,0.00010980031,0.00034547102,0.00014409723,0.0002501417,0.00030816585,0.00014270442,0.00044299904],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012135966,0.000029093339,0.93135196,0.000021241238,0.000015182584,0.0002586257,0.00034024345,0.00021318407,0.06313278,0.000104621664,0.0004684866,0.0039431723],"study_design_scores_gemma":[0.0000012926646,0.000011243837,0.99837315,0.000001783372,0.000004909048,0.00013988039,0.00009344429,0.0002117304,0.00087699783,0.000011555903,0.00027219616,0.0000018457821],"about_ca_topic_score_codex":0.0139182275,"about_ca_topic_score_gemma":0.043615706,"teacher_disagreement_score":0.0139182275,"about_ca_system_score_codex":0.00037680916,"about_ca_system_score_gemma":0.00011450062,"threshold_uncertainty_score":0.027674437},"labels":[],"label_agreement":null},{"id":"W2025016837","doi":"10.1086/341115","title":"<i>r</i>‐Modes in the Ocean of a Magnetic Neutron Star","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Magnetic field; Magnetohydrodynamic drive; L-shell; Shell (structure); Magnetohydrodynamics; Mechanics; Classical mechanics; Earth's magnetic field; Quantum mechanics","score_opus":0.014619369211617123,"score_gpt":0.2801852770833149,"score_spread":0.2655659078716978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025016837","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936993,0.00008859409,0.003872911,0.00008364243,0.000011673933,0.0000043477517,0.00001548679,0.00002965499,0.002194347],"genre_scores_gemma":[0.9980579,0.00007467397,0.0012203685,0.000015369453,0.000007466738,0.0000041786143,0.000022593726,0.000016719987,0.00058075396],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996686,0.0000085173,0.0000017777505,0.000005790783,0.0000059947038,0.000011113358],"domain_scores_gemma":[0.99985933,0.000023601053,0.000053128453,0.00001032958,0.00002012312,0.000033422104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019087722,0.0002521848,0.00021670743,0.00033496734,0.00032434773,0.00043594628,0.00026257557,0.00035376643,0.0005338404],"category_scores_gemma":[0.0005989884,0.00019983276,0.000245854,0.00016447094,0.0006015916,0.00047008964,0.0005252766,0.00028592054,0.00010179015],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005824091,0.00016629476,0.09627023,0.00016549548,0.00011391434,0.001433616,0.0011908358,0.76978564,0.06783658,0.047602013,0.0010078945,0.013845076],"study_design_scores_gemma":[0.0000492668,0.00010248145,0.017998427,0.000015093339,0.000017355704,0.00010630491,0.00025948178,0.971753,0.0030979095,0.005873159,0.0007012555,0.000026284797],"about_ca_topic_score_codex":0.0043520825,"about_ca_topic_score_gemma":0.001457217,"teacher_disagreement_score":0.0043520825,"about_ca_system_score_codex":0.00028928882,"about_ca_system_score_gemma":0.00023092116,"threshold_uncertainty_score":0.008653522},"labels":[],"label_agreement":null},{"id":"W2025052504","doi":"10.1088/0004-637x/797/1/30","title":"CHONDRULE DESTRUCTION IN NEBULAR SHOCKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Chondrule; Planetesimal; Meteorite; Physics; Formation and evolution of the Solar System; Astrophysics; Chondrite; Shock wave; Shock (circulatory); Astrobiology; Solar System; Mechanics","score_opus":0.004928068576376031,"score_gpt":0.1963603971244938,"score_spread":0.19143232854811776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025052504","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99355,0.00040841068,0.0041156146,0.000025047742,0.0000059636695,0.000015370191,0.00009708924,0.000058365236,0.0017242206],"genre_scores_gemma":[0.99836797,0.00016860435,0.00047885493,0.0000118115295,0.0000035070493,0.0000075633234,0.00014041107,0.000011750612,0.00080970774],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980634,0.000018713488,0.0000125163315,0.000053225696,0.000050403265,0.000058793514],"domain_scores_gemma":[0.99964285,0.000096908734,0.00012300389,0.000030210049,0.000033243545,0.00007381869],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026093744,0.00028474454,0.00045866167,0.0003742094,0.00033151841,0.00086346304,0.0004908565,0.00044363507,0.0016635053],"category_scores_gemma":[0.0011093329,0.00018121599,0.0002981983,0.00024369154,0.00037739915,0.00033265914,0.0006432799,0.00027700805,0.00024576564],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011418479,0.00023683782,0.21060258,0.00046991798,0.00029746912,0.003816472,0.00054971944,0.26877642,0.4475281,0.035549294,0.0009355882,0.030095754],"study_design_scores_gemma":[0.00012746964,0.0005678472,0.196595,0.000051830597,0.00012655441,0.002472418,0.000521976,0.6504215,0.12756805,0.018234188,0.0032472922,0.00006592787],"about_ca_topic_score_codex":0.0022013308,"about_ca_topic_score_gemma":0.0008653483,"teacher_disagreement_score":0.0022013308,"about_ca_system_score_codex":0.0007724373,"about_ca_system_score_gemma":0.00020215526,"threshold_uncertainty_score":0.0056043863},"labels":[],"label_agreement":null},{"id":"W2025085301","doi":"10.1086/529581","title":"Probing the Turbulence Dissipation Range and Magnetic Field Strengths in Molecular Clouds","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Molecular cloud; Magnetic field; Turbulence; Dissipation; Spectral line; Decoupling (probability); Range (aeronautics); Ion","score_opus":0.007106130851152405,"score_gpt":0.22496258991827983,"score_spread":0.21785645906712742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025085301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999564,0.00003907377,0.00023716094,0.000007722103,5.248157e-7,7.3005117e-7,0.000009266711,0.0000032094908,0.00013834622],"genre_scores_gemma":[0.9997906,0.000021647053,0.00014709414,0.0000023683178,0.0000015744863,6.9679965e-7,0.0000122009815,0.000001300598,0.000022570614],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999651,0.0000039148263,0.0000015743916,0.000008396519,0.0000073066635,0.000013758129],"domain_scores_gemma":[0.999724,0.00008696094,0.00010736431,0.000014742354,0.000019919713,0.000047071717],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010251654,0.0001813171,0.00015607936,0.0004857097,0.00023269837,0.00027253345,0.0001490781,0.00012964467,0.00025224467],"category_scores_gemma":[0.0005077244,0.000120663906,0.00008908008,0.00029280168,0.00029679743,0.0002853748,0.00029733585,0.00022760323,0.000041692172],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006347774,0.00012876905,0.2780608,0.000051566425,0.000084785795,0.0003112043,0.00051361514,0.013763932,0.6925853,0.00198656,0.00008543456,0.01179336],"study_design_scores_gemma":[0.000090650035,0.0004585523,0.78623426,0.000018582192,0.00007419774,0.00040948618,0.00037950856,0.090088755,0.119811,0.0018124494,0.0005698593,0.00005270397],"about_ca_topic_score_codex":0.0014627228,"about_ca_topic_score_gemma":0.0016006762,"teacher_disagreement_score":0.0014627228,"about_ca_system_score_codex":0.00018709234,"about_ca_system_score_gemma":0.000087625245,"threshold_uncertainty_score":0.002908349},"labels":[],"label_agreement":null},{"id":"W2025097755","doi":"10.1086/318423","title":"The Evolution of Population Gradients in Galaxy Clusters: The Butcher‐Oemler Effect and Cluster Infall","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":248,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Galaxy; Astronomy; Redshift; Population; Luminosity; Galaxy cluster; Star formation; RADIUS; Cluster (spacecraft); Galaxy formation and evolution","score_opus":0.004782931825303339,"score_gpt":0.211820380882205,"score_spread":0.20703744905690166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025097755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99934644,0.00012838445,0.00011522321,0.000042368847,0.0000011278389,0.0000013379886,0.000059508086,0.000008541338,0.00029715055],"genre_scores_gemma":[0.9997805,0.00001971491,0.00005350285,0.0000076569995,0.00000389183,8.3588867e-7,0.00006373405,0.00000304012,0.000067157285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996112,0.000083149156,0.000021714888,0.00012539844,0.00006185376,0.00009669556],"domain_scores_gemma":[0.99552,0.0015513052,0.0017464778,0.00043021486,0.00021632212,0.00053565216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000721196,0.00015309645,0.00025915282,0.0011454005,0.00039621413,0.0006082411,0.00031025714,0.00040404734,0.0011594297],"category_scores_gemma":[0.0045886682,0.00015068661,0.0002233793,0.0006286312,0.00079584133,0.00072961947,0.0007191577,0.0002932495,0.00015827254],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012564074,0.000011094616,0.99389935,0.000004885126,0.000042069652,0.00006226617,0.00022409357,0.00038043808,0.0024764903,0.0002881903,0.00009273528,0.002392774],"study_design_scores_gemma":[0.000001571987,0.000015003417,0.9990778,8.2204605e-7,0.0000061223977,0.000046495465,0.0000382847,0.00049143884,0.00016753931,0.0000757847,0.00007615964,0.0000030586702],"about_ca_topic_score_codex":0.007029507,"about_ca_topic_score_gemma":0.007991495,"teacher_disagreement_score":0.007029507,"about_ca_system_score_codex":0.00046089556,"about_ca_system_score_gemma":0.00012902226,"threshold_uncertainty_score":0.01397717},"labels":[],"label_agreement":null},{"id":"W2025147054","doi":"10.1086/422911","title":"Green Bank Telescope Measurement of the Systemic Velocity of the Double Pulsar Binary J0737-3039 and Implications for Its Formation","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Natural Sciences and Engineering Research Council of Canada; McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Green Bank Telescope; Radio telescope; Telescope; Sky; Binary pulsar; Binary number; Astronomy; Scintillation; Millisecond pulsar; Optics; Detector","score_opus":0.029617260995810475,"score_gpt":0.3029108454508083,"score_spread":0.27329358445499785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025147054","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99716717,0.00017312662,0.00047396065,0.00005646952,0.000012034985,0.0000071251225,0.00039244522,0.000035802932,0.0016817608],"genre_scores_gemma":[0.9976035,0.00010421474,0.0012996622,0.000034484336,0.000011027228,0.000008913726,0.00063754764,0.0000073481206,0.00029325834],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985635,0.000016497886,0.0000068976387,0.000036091787,0.00004672473,0.00003740339],"domain_scores_gemma":[0.9996402,0.000043958684,0.00010008963,0.000043264256,0.0000676171,0.000104855324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002500296,0.00015646484,0.00022602691,0.00063797424,0.0005676256,0.00040328735,0.00027708308,0.00031210302,0.0007661329],"category_scores_gemma":[0.00052740425,0.0001951796,0.00013911909,0.0005826023,0.00031089608,0.00024985446,0.0004968743,0.0003493305,0.0005030516],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045933248,0.00012607586,0.7172525,0.00007063823,0.00006936484,0.0006542616,0.0005599074,0.0014148301,0.25266826,0.0015771654,0.0023090092,0.022838667],"study_design_scores_gemma":[0.00004985513,0.0001703122,0.97316235,0.000016927012,0.000042113235,0.00079893327,0.00016467649,0.004705225,0.016943026,0.0003903288,0.0035232913,0.0000328304],"about_ca_topic_score_codex":0.009895288,"about_ca_topic_score_gemma":0.019944934,"teacher_disagreement_score":0.009895288,"about_ca_system_score_codex":0.0005307758,"about_ca_system_score_gemma":0.00055749604,"threshold_uncertainty_score":0.019675374},"labels":[],"label_agreement":null},{"id":"W2025166677","doi":"10.1088/0004-637x/778/1/57","title":"QUANTIFYING MASS SEGREGATION AND NEW CORE RADII FOR 54 MILKY WAY GLOBULAR CLUSTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"Globular cluster; Milky Way; Astrophysics; Physics; Cluster (spacecraft); RADIUS; Mass segregation; Star cluster; Power law; Open cluster; Surface brightness; Stars; Core (optical fiber); Statistics; Galaxy; Mathematics","score_opus":0.03542168562313887,"score_gpt":0.25414598770995417,"score_spread":0.21872430208681531,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025166677","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99955887,0.00004416314,0.0002228719,0.000003830892,3.6546663e-7,0.0000016655044,0.000060328803,0.000011204271,0.00009666477],"genre_scores_gemma":[0.99874926,0.000041150455,0.000656774,0.000002959283,0.0000012982958,0.000004382025,0.00039281452,0.000016199883,0.00013514877],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996985,0.0000416503,0.000025695197,0.000121414596,0.000060757946,0.000051980922],"domain_scores_gemma":[0.9980172,0.000628059,0.00056343264,0.000261059,0.00028918264,0.00024104347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001098764,0.00033864463,0.00051848404,0.0027993133,0.00051528093,0.00077940285,0.0005475967,0.00041737207,0.0007482126],"category_scores_gemma":[0.0050095473,0.0002857862,0.0005232455,0.0014014263,0.0005129138,0.0005721235,0.001218122,0.00024077391,0.0002511729],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026615846,0.000016335262,0.96847737,0.000032076663,0.00013678364,0.000091423935,0.00087776105,0.01261393,0.010449489,0.0004942176,0.00019292216,0.0063514677],"study_design_scores_gemma":[0.000010987465,0.00005318775,0.9726668,0.000010431472,0.00005758552,0.00014554324,0.00041892537,0.021978285,0.0035371312,0.00043136367,0.0006663246,0.00002336627],"about_ca_topic_score_codex":0.00944155,"about_ca_topic_score_gemma":0.01275959,"teacher_disagreement_score":0.00944155,"about_ca_system_score_codex":0.0010461026,"about_ca_system_score_gemma":0.00023345416,"threshold_uncertainty_score":0.018773198},"labels":[],"label_agreement":null},{"id":"W2025243492","doi":"10.1088/0004-637x/788/1/65","title":"IMPROVED DETERMINATION OF THE ATMOSPHERIC PARAMETERS OF THE PULSATING sdB STAR FEIGE 48","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Effective temperature; Blanketing; Surface gravity; Atmosphere (unit); Spectral line; Line (geometry); Star (game theory); Opacity; Stellar atmosphere","score_opus":0.007315908437413852,"score_gpt":0.20761527472762847,"score_spread":0.2002993662902146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025243492","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99037474,0.000078221216,0.00758914,0.000051186133,0.0000074964464,0.000007712879,0.0007842611,0.00028035237,0.00082685036],"genre_scores_gemma":[0.9888559,0.000035628214,0.009744864,0.000013232193,0.000010046726,0.00001093164,0.0011371705,0.00004772509,0.00014454026],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998418,0.000025296982,0.000010069586,0.00006849703,0.000032547458,0.000021776708],"domain_scores_gemma":[0.9996872,0.0000663354,0.000041858206,0.00010110756,0.00005714037,0.00004649792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002853579,0.0004120735,0.00047227202,0.0007455943,0.00033843052,0.00060075393,0.0006805887,0.00047502495,0.000866667],"category_scores_gemma":[0.0010967066,0.000341958,0.0005387073,0.00039274446,0.00014769446,0.0005362772,0.0006381615,0.00053567946,0.0003625474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029674685,0.0002782616,0.7204599,0.000095547046,0.00018426572,0.00040115134,0.00053706707,0.08581165,0.14374101,0.0011416639,0.0009708858,0.046081953],"study_design_scores_gemma":[0.00011365559,0.00013475688,0.65627563,0.000031962725,0.00009304243,0.00035060523,0.00017196822,0.31840175,0.018391078,0.0015816112,0.0043961327,0.00005785417],"about_ca_topic_score_codex":0.0037665875,"about_ca_topic_score_gemma":0.0038995894,"teacher_disagreement_score":0.0037665875,"about_ca_system_score_codex":0.00035395214,"about_ca_system_score_gemma":0.00021297709,"threshold_uncertainty_score":0.0074893236},"labels":[],"label_agreement":null},{"id":"W2025281695","doi":"10.1086/422829","title":"Self‐Calibration in Cluster Studies of Dark Energy: Combining the Cluster Redshift Distribution, the Power Spectrum, and Mass Measurements","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":219,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Redshift; Dark energy; Cluster (spacecraft); Cosmic microwave background; Galaxy cluster; Spectral density; Context (archaeology); Photometric redshift; Galaxy","score_opus":0.011923369117859977,"score_gpt":0.22413316539699077,"score_spread":0.21220979627913078,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025281695","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93209064,0.0007576264,0.062289745,0.00028688266,0.00001918593,0.000030727,0.0001572668,0.00014953088,0.00421832],"genre_scores_gemma":[0.97873116,0.00021608762,0.020476488,0.000066286804,0.000027382135,0.00001942551,0.00015680908,0.00004076403,0.00026555388],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.998166,0.0008903269,0.00007507266,0.00034262284,0.00040241334,0.00012356704],"domain_scores_gemma":[0.98687416,0.0053316737,0.0027159282,0.003842662,0.00088859623,0.00034694147],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005875961,0.0007019409,0.0005847199,0.00371692,0.00062261045,0.0018873152,0.0010256002,0.0006227363,0.00043421306],"category_scores_gemma":[0.016779525,0.0005183536,0.00059773686,0.004012671,0.0014249247,0.0030981943,0.0041771093,0.0009359412,0.00020349196],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014126791,0.00008944705,0.8858153,0.00009095126,0.00041246417,0.00022260216,0.00093514164,0.024250034,0.007580794,0.012451189,0.0004207834,0.06759005],"study_design_scores_gemma":[0.000029617442,0.00015370024,0.7979464,0.00007377263,0.00014796806,0.00049632695,0.0006902157,0.13422006,0.015431811,0.04674059,0.0039143115,0.00015521805],"about_ca_topic_score_codex":0.0053770905,"about_ca_topic_score_gemma":0.0092195785,"teacher_disagreement_score":0.005875961,"about_ca_system_score_codex":0.0006383826,"about_ca_system_score_gemma":0.00046245658,"threshold_uncertainty_score":0.031075418},"labels":[],"label_agreement":null},{"id":"W2025312248","doi":"10.1086/308456","title":"Space Telescope Imaging Spectrograph Long‐Slit Spectroscopy of the Narrow‐Line Region of NGC 4151. I. Kinematics and Emission‐Line Ratios","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Outflow; Space Telescope Imaging Spectrograph; Kinematics; Galaxy; Spectroscopy; Spectral line; Line (geometry); Very Large Telescope; Emission spectrum","score_opus":0.005720156893523643,"score_gpt":0.21674529252241806,"score_spread":0.2110251356288944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025312248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.987571,0.00026680794,0.0005426752,0.00010538273,0.000014145671,0.000031292806,0.005787771,0.0002285429,0.0054523423],"genre_scores_gemma":[0.9807535,0.00026783184,0.002464101,0.00014519136,0.000024108404,0.000035025838,0.01147161,0.000036179823,0.0048024915],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998841,0.000008925927,0.000009300414,0.000034234432,0.000037320875,0.000026124608],"domain_scores_gemma":[0.99961084,0.00002487122,0.00014640186,0.000048374626,0.00007046096,0.00009904591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026657546,0.0002637674,0.00018932005,0.0013850287,0.0006150749,0.00043422738,0.00023496707,0.00026358388,0.0031715776],"category_scores_gemma":[0.00025337972,0.0001704024,0.00018419544,0.00086258893,0.00012884742,0.00030926132,0.0003295169,0.00028220136,0.00071791175],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055822975,0.00028511422,0.7501148,0.00022649666,0.0002045661,0.0010672647,0.0013837932,0.00063325185,0.20371476,0.0005609052,0.007462549,0.033788286],"study_design_scores_gemma":[0.000007498623,0.00005584732,0.9953974,0.0000059306262,0.00002403251,0.00019278454,0.00009782524,0.00018310477,0.0019488198,0.000041039464,0.0020414235,0.0000043638624],"about_ca_topic_score_codex":0.007220328,"about_ca_topic_score_gemma":0.018888876,"teacher_disagreement_score":0.007220328,"about_ca_system_score_codex":0.00035496167,"about_ca_system_score_gemma":0.00015283187,"threshold_uncertainty_score":0.014356613},"labels":[],"label_agreement":null},{"id":"W2025367319","doi":"10.1088/0004-637x/756/2/145","title":"ASPECT RATIO DEPENDENCE OF THE FREE-FALL TIME FOR NON-SPHERICAL SYMMETRIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Aspect ratio (aeronautics); Enhanced Data Rates for GSM Evolution; Homogeneous space; Acceleration; Square root; SPHERES; Square (algebra); Mode (computer interface)","score_opus":0.009905060061131213,"score_gpt":0.23359165167518323,"score_spread":0.22368659161405202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025367319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97374785,0.00052889594,0.019462505,0.00013110631,0.0000187932,0.000016614878,0.00015157327,0.00015792556,0.005784718],"genre_scores_gemma":[0.9975228,0.00010333623,0.0019676453,0.000007977688,0.0000041907483,0.0000047482013,0.00009963123,0.00003966505,0.00024992885],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998878,0.000010424941,0.0000055643923,0.000026393936,0.000032435975,0.000037343085],"domain_scores_gemma":[0.99907947,0.0003803974,0.00030910343,0.000061191124,0.0000688434,0.00010098212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032575277,0.00035864022,0.00023873623,0.00072602276,0.00031304738,0.00046474545,0.0005921808,0.00027852046,0.0018606208],"category_scores_gemma":[0.0027980465,0.00013817093,0.00042076607,0.00028173844,0.00051891024,0.0005880727,0.00033931507,0.0003863528,0.0002674999],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005417596,0.00021100638,0.10650295,0.0002965635,0.00014077527,0.0021431209,0.0005350686,0.56917536,0.21941113,0.058816124,0.0014863367,0.040739838],"study_design_scores_gemma":[0.000020397409,0.00007665097,0.028859228,0.000011722421,0.000022502014,0.00044428546,0.000049504833,0.9395641,0.019774688,0.010709297,0.00043095948,0.000036516572],"about_ca_topic_score_codex":0.0023997233,"about_ca_topic_score_gemma":0.001964897,"teacher_disagreement_score":0.0023997233,"about_ca_system_score_codex":0.0005321608,"about_ca_system_score_gemma":0.00024870032,"threshold_uncertainty_score":0.006224394},"labels":[],"label_agreement":null},{"id":"W2025501883","doi":"10.1086/375798","title":"The Contribution of Particle Impact to the Production of Fe Kα Emission from Accreting Black Holes","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Electron; Astrophysics; Accretion (finance); Photoionization; Flux (metallurgy); Particle acceleration; Solar flare; Context (archaeology); Atomic physics; Computational physics; Nuclear physics; Ion; Ionization; Chemistry","score_opus":0.012846830585896939,"score_gpt":0.25715766609763957,"score_spread":0.24431083551174262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025501883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960573,0.00068021816,0.0018277233,0.000048833917,0.000011733035,0.000010889683,0.000021349591,0.000025724537,0.0013162105],"genre_scores_gemma":[0.9992095,0.0002822586,0.00017799501,0.000011179012,0.0000132678,0.0000030952924,0.00004002148,0.0000073274127,0.00025533471],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999821,0.00003856667,0.000009846143,0.00004302785,0.00003929011,0.000048236812],"domain_scores_gemma":[0.9994066,0.0003285088,0.000107350694,0.00004920355,0.000045415065,0.00006296052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004679702,0.00081809604,0.00039932595,0.0005942536,0.00039135825,0.0009515084,0.0004908803,0.0006333101,0.0009996559],"category_scores_gemma":[0.0015803063,0.00042554492,0.00039696932,0.00021908229,0.00064799207,0.000437681,0.00070176536,0.00034419168,0.00020930235],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002971434,0.00031691973,0.49359566,0.0006554625,0.0005283162,0.009386354,0.000779976,0.05141497,0.39716357,0.004687897,0.00031168247,0.038187683],"study_design_scores_gemma":[0.00014962147,0.0011326536,0.7438868,0.000044413402,0.00030825086,0.003252968,0.0004602123,0.10175573,0.1416136,0.0058344146,0.0015135548,0.000047722344],"about_ca_topic_score_codex":0.0007693505,"about_ca_topic_score_gemma":0.00027747723,"teacher_disagreement_score":0.0009996559,"about_ca_system_score_codex":0.000395035,"about_ca_system_score_gemma":0.00019037865,"threshold_uncertainty_score":0.0033441782},"labels":[],"label_agreement":null},{"id":"W2025551781","doi":"10.1086/426474","title":"Toward an Improved Analytical Description of Lagrangian Bias","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Queen's University","funders":"","keywords":"Redshift; Eulerian path; Lagrangian; Distribution (mathematics); Distribution function; Function (biology); Correlation function (quantum field theory); Mass distribution","score_opus":0.024242082305958174,"score_gpt":0.2342173686954114,"score_spread":0.20997528638945323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025551781","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.11453183,0.0008468246,0.8702038,0.0009192607,0.00007166118,0.000050740327,0.0001660044,0.00041368074,0.01279615],"genre_scores_gemma":[0.8397393,0.0012678856,0.15159886,0.00040249457,0.00022708836,0.00013633822,0.00012945461,0.0003991059,0.006099388],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.999522,0.00016863931,0.000021878071,0.000053364798,0.00015184017,0.000082319],"domain_scores_gemma":[0.99811894,0.00070610794,0.00045071423,0.0002717218,0.00035571086,0.00009670962],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022154588,0.00058647856,0.0006534545,0.0013333687,0.00045080562,0.0011352353,0.0018245495,0.0007189753,0.002129745],"category_scores_gemma":[0.01327691,0.00038665973,0.00070510746,0.0010019529,0.0009460362,0.0028430044,0.00156879,0.0008457771,0.0005357073],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002039578,0.00003260486,0.007850454,0.00006799884,0.000030167079,0.0001887741,0.00018520006,0.50877523,0.0022443535,0.46708214,0.0010105135,0.0125121735],"study_design_scores_gemma":[0.0000065434383,0.0000078661715,0.00049884623,0.0000108308395,0.000004388643,0.000027869706,0.0000103893,0.9469582,0.0002602321,0.051122252,0.0010808709,0.000011730704],"about_ca_topic_score_codex":0.006273843,"about_ca_topic_score_gemma":0.0035324874,"teacher_disagreement_score":0.006273843,"about_ca_system_score_codex":0.0016573116,"about_ca_system_score_gemma":0.0013581696,"threshold_uncertainty_score":0.012474656},"labels":[],"label_agreement":null},{"id":"W2025595361","doi":"10.1086/339060","title":"Stellar Collisions and the Interior Structure of Blue Stragglers","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Smoothed-particle hydrodynamics; Physics; Stars; Simple (philosophy); Globular cluster; Statistical physics; Astrophysics; Stellar collision; Mixing (physics); Blue straggler; Star cluster; Stellar evolution; Angular momentum; Computer science; Classical mechanics","score_opus":0.00865737711575456,"score_gpt":0.21650140051693603,"score_spread":0.20784402340118147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025595361","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965642,0.00022927039,0.0015713666,0.000036471865,0.0000037490286,0.0000022135455,0.000019324767,0.000055649565,0.0015176215],"genre_scores_gemma":[0.9987772,0.00008964077,0.0004730028,0.0000122627325,0.0000036686074,0.0000011887165,0.00005096542,0.000022805518,0.00056920026],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999548,0.0000085414695,0.0000015397909,0.000008442135,0.000010271076,0.000016373748],"domain_scores_gemma":[0.99971575,0.00004055783,0.00011211808,0.000017958766,0.000029005283,0.000084646985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013591135,0.00018181016,0.00029039333,0.00054265466,0.0006734549,0.0010683195,0.00036191114,0.00041217706,0.0011393608],"category_scores_gemma":[0.00082821964,0.0003054124,0.00014593269,0.00031271926,0.00078779884,0.00044563814,0.0009288091,0.00032232617,0.00036347384],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013319944,0.00031351869,0.41565055,0.00015268158,0.0001616627,0.003128665,0.0041930494,0.29554245,0.12248596,0.114706516,0.004327445,0.03800556],"study_design_scores_gemma":[0.00018220197,0.00025675885,0.28938925,0.00007097426,0.00006588481,0.001821934,0.0013735153,0.61422706,0.021054255,0.062603354,0.008836143,0.000118744974],"about_ca_topic_score_codex":0.003171306,"about_ca_topic_score_gemma":0.0021301575,"teacher_disagreement_score":0.003171306,"about_ca_system_score_codex":0.00047924902,"about_ca_system_score_gemma":0.00022625567,"threshold_uncertainty_score":0.0063056946},"labels":[],"label_agreement":null},{"id":"W2025612492","doi":"10.1088/0004-637x/735/1/66","title":"RADIATION PRESSURE FROM MASSIVE STAR CLUSTERS AS A LAUNCHING MECHANISM FOR SUPER-GALACTIC WINDS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":252,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Supernova; Radiation pressure; Galaxy; Star formation; Star cluster; Radiation; Ram pressure","score_opus":0.009978930726492943,"score_gpt":0.20717740466030768,"score_spread":0.19719847393381473,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025612492","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98261815,0.0006588413,0.004967966,0.00019340565,0.000049167433,0.000026748243,0.000093029026,0.00025929057,0.011133289],"genre_scores_gemma":[0.997712,0.00013303882,0.00054822443,0.000030811374,0.000016540213,0.000006059186,0.00005025698,0.0000110033725,0.0014920082],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999249,0.000008398088,0.0000032010682,0.000017612258,0.000015319227,0.000030455494],"domain_scores_gemma":[0.9997485,0.000038211045,0.00008007038,0.00002743789,0.000021318983,0.000084344436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015217792,0.00034984143,0.00027034382,0.00023168333,0.00038715155,0.00071171345,0.00062060007,0.0005162223,0.0031433874],"category_scores_gemma":[0.00028962106,0.00018037233,0.0003593771,0.00014150213,0.0002805066,0.00044257523,0.00052320265,0.00043070732,0.0006698891],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008045404,0.00037623566,0.4216275,0.00044130813,0.0002723988,0.0077414294,0.0009897875,0.06895904,0.39001307,0.069421664,0.005125398,0.03422755],"study_design_scores_gemma":[0.00033490596,0.0013635557,0.67503715,0.00009750057,0.00022544514,0.0040661185,0.0010078873,0.22590338,0.046401154,0.024079382,0.021298349,0.0001851888],"about_ca_topic_score_codex":0.001706524,"about_ca_topic_score_gemma":0.0013202211,"teacher_disagreement_score":0.0031433874,"about_ca_system_score_codex":0.00053331885,"about_ca_system_score_gemma":0.00021216676,"threshold_uncertainty_score":0.010515749},"labels":[],"label_agreement":null},{"id":"W2025616764","doi":"10.1086/312610","title":"L1551NE—Discovery of a Binary Companion","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Circumbinary planet; Astrophysics; Protostar; Physics; Circumstellar envelope; Millimeter; Binary number; Astronomy; Primary (astronomy); Star formation; Stars","score_opus":0.009410339752777287,"score_gpt":0.2324767702360238,"score_spread":0.22306643048324654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025616764","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959137,0.00037289457,0.00024121975,0.000045889217,0.000016550079,0.000007406815,0.00011076247,0.000016249502,0.0032752883],"genre_scores_gemma":[0.9984144,0.00007119731,0.00032642373,0.000050859424,0.000010570481,0.0000026302075,0.00020722652,0.000002423435,0.00091420114],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.000007699814,0.0000076230076,0.000050078346,0.000025644464,0.000026769472],"domain_scores_gemma":[0.9997639,0.000023606386,0.000060593295,0.00002647269,0.00003036122,0.000095068885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021602603,0.00013074499,0.00024233472,0.0005563868,0.0007263553,0.0006332823,0.0002868136,0.000529799,0.0014943399],"category_scores_gemma":[0.00041454367,0.00014053559,0.0001375978,0.00016671683,0.00025952174,0.00026198593,0.00065576914,0.00032459304,0.00061616296],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046736273,0.00024900114,0.59096056,0.00015392259,0.00008925414,0.009237994,0.0015566119,0.00023700131,0.35584316,0.0019055918,0.0020579048,0.037241686],"study_design_scores_gemma":[0.000018901823,0.0003848303,0.95572764,0.00004010184,0.000034888664,0.010100507,0.0005538576,0.0004980796,0.017636266,0.00031885636,0.01466647,0.000019642512],"about_ca_topic_score_codex":0.0017659974,"about_ca_topic_score_gemma":0.0025234038,"teacher_disagreement_score":0.0017659974,"about_ca_system_score_codex":0.00049466005,"about_ca_system_score_gemma":0.00013867884,"threshold_uncertainty_score":0.004999101},"labels":[],"label_agreement":null},{"id":"W2025698758","doi":"10.1088/0004-637x/772/2/130","title":"ON THE FORM OF THE<i>SPITZER</i>LEAVITT LAW AND ITS DEPENDENCE ON METALLICITY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Cepheid variable; Metallicity; Astrophysics; Physics; Period (music); Magnitude (astronomy); Galaxy; Stars","score_opus":0.011697945932811262,"score_gpt":0.2107930502039844,"score_spread":0.19909510427117313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025698758","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.33756676,0.008107224,0.28854445,0.018053133,0.0006551841,0.00017674455,0.0027415245,0.004179897,0.33997512],"genre_scores_gemma":[0.9523105,0.002775846,0.027620414,0.001208509,0.00032240525,0.00007206152,0.0008315697,0.0013072813,0.013551391],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99961853,0.00008243796,0.000023652481,0.00010864981,0.0001258395,0.000040981122],"domain_scores_gemma":[0.9970241,0.0012121936,0.0006106079,0.00056956126,0.0004809034,0.00010266677],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012775607,0.00033548794,0.00032977117,0.0013324413,0.00044605762,0.003046443,0.0017561602,0.0006652549,0.008264228],"category_scores_gemma":[0.011261018,0.000267884,0.0004497056,0.0013455988,0.001906816,0.0029510888,0.0007318318,0.0017385109,0.0023583411],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027000246,0.0000789598,0.09159214,0.00055154983,0.00012685065,0.00050506205,0.0016651631,0.009189838,0.01657149,0.66402686,0.022153364,0.19326888],"study_design_scores_gemma":[0.000053024665,0.00030487872,0.26619974,0.0006495637,0.0001268093,0.0013154813,0.0014432216,0.066898,0.016310085,0.49991918,0.14659086,0.00018910882],"about_ca_topic_score_codex":0.003808494,"about_ca_topic_score_gemma":0.0024703343,"teacher_disagreement_score":0.008264228,"about_ca_system_score_codex":0.00088521506,"about_ca_system_score_gemma":0.00040999503,"threshold_uncertainty_score":0.027646542},"labels":[],"label_agreement":null},{"id":"W2025929644","doi":"10.1088/0004-637x/748/2/131","title":"ON THE LINK BETWEEN ASSOCIATED Mg II ABSORBERS AND STAR FORMATION IN QUASAR HOSTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Quasar; OVV quasar; Galaxy; Star formation; Population; Emission spectrum","score_opus":0.01130793942040771,"score_gpt":0.2195914138268267,"score_spread":0.208283474406419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2025929644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987658,0.00021733853,0.000058819263,0.000054636006,0.000002525548,0.0000015868316,0.000068838075,0.00000389673,0.00082659157],"genre_scores_gemma":[0.999723,0.000052461393,0.000024836749,0.0000121928415,0.000009445181,8.1938646e-7,0.000065822984,0.0000012788416,0.000110075795],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978524,0.000056048422,0.00001704791,0.000050939503,0.000025368749,0.00006533168],"domain_scores_gemma":[0.99533075,0.0017918043,0.0016196923,0.00016672544,0.00017255351,0.0009184499],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048260912,0.00017650514,0.00017349649,0.0012860488,0.0002803101,0.00078985805,0.0003326084,0.00057408755,0.0050541633],"category_scores_gemma":[0.002904812,0.00015242698,0.00017284938,0.0008289764,0.000483184,0.0005341132,0.0004024528,0.00036077522,0.00047707857],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000072050534,0.000025410533,0.99786264,0.000004680249,0.000022646704,0.00008673019,0.00004383384,0.000046340123,0.00092042447,0.00009085996,0.000034967386,0.0007894389],"study_design_scores_gemma":[0.000002012367,0.00004039901,0.99939823,0.0000028653433,0.000011919625,0.00012596112,0.000078431905,0.00013856767,0.0000762929,0.00005833525,0.00006568686,0.0000013754362],"about_ca_topic_score_codex":0.0016907357,"about_ca_topic_score_gemma":0.002146937,"teacher_disagreement_score":0.0050541633,"about_ca_system_score_codex":0.00012699894,"about_ca_system_score_gemma":0.00012254248,"threshold_uncertainty_score":0.01690793},"labels":[],"label_agreement":null},{"id":"W2026030071","doi":"10.1086/511259","title":"Direct Measurement of the Ratio of Carbon Monoxide to Molecular Hydrogen in the Diffuse Interstellar Medium","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":157,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Excitation temperature; Interstellar medium; Physics; Hydrogen; Molecular cloud; Spectral line; Analytical Chemistry (journal); Carbon monoxide; Ultraviolet; Stars; Atomic physics; Emission spectrum; Chemistry; Astronomy; Galaxy; Optics","score_opus":0.011256691628566795,"score_gpt":0.22739307315325602,"score_spread":0.21613638152468923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026030071","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971488,0.00023646001,0.0006552995,0.000006153348,0.000002469188,0.000006153395,0.0004978562,0.000024362414,0.0014224097],"genre_scores_gemma":[0.99754673,0.00015568126,0.00096487167,0.000012022814,0.0000052699393,0.000006629916,0.00073554437,0.0000052099685,0.0005680999],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998609,0.000007536149,0.00000429491,0.000068992194,0.00003485235,0.000023525248],"domain_scores_gemma":[0.9998542,0.000018764802,0.0000258933,0.000019813722,0.00003208521,0.000049234983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012546821,0.00025214994,0.00013454222,0.00097419234,0.00030286395,0.00048014024,0.00028919452,0.00021773679,0.0012471356],"category_scores_gemma":[0.0002803924,0.00016648236,0.0000923806,0.00048703497,0.0002447977,0.00032172687,0.00039642624,0.00022963563,0.00027484063],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026437407,0.00011597197,0.4792023,0.00006420591,0.00014101551,0.00012490767,0.00025855345,0.0004084322,0.5061641,0.0002537132,0.00018503446,0.01281749],"study_design_scores_gemma":[0.000010063625,0.0001867366,0.9292199,0.0000060419106,0.00003649685,0.00034790373,0.00020731371,0.0013094504,0.067239396,0.000073022005,0.0013526129,0.000011048873],"about_ca_topic_score_codex":0.003599219,"about_ca_topic_score_gemma":0.00835654,"teacher_disagreement_score":0.003599219,"about_ca_system_score_codex":0.00021144541,"about_ca_system_score_gemma":0.00011179361,"threshold_uncertainty_score":0.007156551},"labels":[],"label_agreement":null},{"id":"W2026058600","doi":"10.1088/0004-637x/800/1/51","title":"AN INFRARED CENSUS OF DUST IN NEARBY GALAXIES WITH<i>SPITZER</i>(DUSTiNGS). II. DISCOVERY OF METAL-POOR DUSTY AGB STARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Physics; Asymptotic giant branch; Astrophysics; Stars; Galaxy; Carbon star; Astronomy; Circumstellar dust; Metallicity; Photometry (optics)","score_opus":0.016417405185430774,"score_gpt":0.23157944450497905,"score_spread":0.21516203931954828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026058600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99002284,0.00016640984,0.00013890715,0.000033441906,0.0000027015283,0.000020689517,0.008414353,0.000031914722,0.0011687126],"genre_scores_gemma":[0.9701489,0.0002764983,0.0010936189,0.00007893379,0.00002803902,0.000040752708,0.026921554,0.000018736297,0.0013930117],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998349,0.000009950779,0.000019727306,0.00005267322,0.000043019005,0.000039590093],"domain_scores_gemma":[0.9991091,0.00005924805,0.00028921728,0.00006827686,0.0001787158,0.00029539224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018633163,0.00018901125,0.0001615073,0.0026511527,0.00025285268,0.00029680677,0.00024979704,0.00020529542,0.0012996874],"category_scores_gemma":[0.0004318542,0.00013882782,0.00017638318,0.0015016119,0.00015550225,0.0003119489,0.00043449647,0.00018247687,0.00060339615],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006038134,0.000034654156,0.9828399,0.000032404867,0.00003014382,0.00014004475,0.00023674997,0.00006838176,0.0075488384,0.000081147205,0.0011859154,0.0077413754],"study_design_scores_gemma":[0.0000010604615,0.000010902074,0.99901927,0.000001327096,0.000003075027,0.000071916715,0.00003426584,0.000035524605,0.00018263729,0.0000057730654,0.00063343137,7.461941e-7],"about_ca_topic_score_codex":0.010628496,"about_ca_topic_score_gemma":0.019630587,"teacher_disagreement_score":0.010628496,"about_ca_system_score_codex":0.0003002108,"about_ca_system_score_gemma":0.00020715536,"threshold_uncertainty_score":0.021133244},"labels":[],"label_agreement":null},{"id":"W2026129840","doi":"10.1088/0004-637x/795/1/71","title":"SURFACE GEOMETRY OF PROTOPLANETARY DISKS INFERRED FROM NEAR-INFRARED IMAGING POLARIMETRY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Protoplanetary disk; Surface (topology); Astrophysics; Planet; Infrared; Spiral galaxy; Maxima; Scattering; Position angle; Geometry; Position (finance); Stars; Optics; Galaxy","score_opus":0.007588641192087207,"score_gpt":0.22965429838052567,"score_spread":0.22206565718843846,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026129840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95793927,0.00020734842,0.03615881,0.000028817047,0.000005788036,0.000039797607,0.0010942089,0.00020860352,0.004317383],"genre_scores_gemma":[0.9730355,0.00009947716,0.02583573,0.0000050983354,0.000008643685,0.000021436768,0.0007702983,0.000022044635,0.00020186117],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990356,0.000013063024,0.0000037501864,0.00003042451,0.000036463687,0.000012782123],"domain_scores_gemma":[0.9998271,0.000034029854,0.000039018472,0.000028324966,0.0000536914,0.000017983715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009093384,0.00027899886,0.00021602068,0.0012367471,0.00023040212,0.00044080816,0.00027778454,0.00012687658,0.00067757705],"category_scores_gemma":[0.00035528108,0.00018188661,0.00023069228,0.00051811873,0.00018196608,0.00036164504,0.00038738584,0.0001692706,0.00022305326],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022640597,0.00006300049,0.62494135,0.00012657455,0.00010057334,0.00036740975,0.0005245289,0.028725907,0.23574132,0.0025930046,0.0006880634,0.105901875],"study_design_scores_gemma":[0.000026857424,0.00006141426,0.8511384,0.000012163927,0.00004596252,0.00050723046,0.00025989173,0.11489392,0.02972618,0.0014315064,0.0018532595,0.00004321684],"about_ca_topic_score_codex":0.0020915212,"about_ca_topic_score_gemma":0.0027558515,"teacher_disagreement_score":0.0020915212,"about_ca_system_score_codex":0.0002780583,"about_ca_system_score_gemma":0.00016457103,"threshold_uncertainty_score":0.0041587353},"labels":[],"label_agreement":null},{"id":"W2026170380","doi":"10.1088/0004-637x/692/1/298","title":"MORPHOLOGICAL COMPOSITION OF<i>z</i>∼ 0.4 GROUPS: THE SITE OF S0 FORMATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Luminosity; Star formation; Redshift; Galaxy formation and evolution; Lenticular galaxy; Elliptical galaxy; Galaxy group","score_opus":0.007751658850945565,"score_gpt":0.21028023853783484,"score_spread":0.20252857968688928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026170380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985719,0.000048930924,0.00007930889,0.00001640194,0.000001264162,0.000003315358,0.00010809044,0.000011194361,0.0011595908],"genre_scores_gemma":[0.99918324,0.000024718829,0.00010098934,0.000009878129,0.0000035323346,0.0000029942817,0.0002696012,0.0000059738727,0.00039907428],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997892,0.000018718649,0.000011792077,0.000055148754,0.000036567217,0.00008862473],"domain_scores_gemma":[0.9991812,0.000055888206,0.0002745918,0.00006543534,0.0001227938,0.00030010196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022242736,0.00017315042,0.00021473106,0.0018998854,0.0003709585,0.00082400773,0.00036194857,0.0002011355,0.0031545444],"category_scores_gemma":[0.00085606374,0.00011710701,0.00019042005,0.000574529,0.0005367144,0.00036913063,0.0007530237,0.00013860401,0.0007784053],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026935784,0.000026523028,0.97923905,0.000014519,0.00003328942,0.00007937806,0.00054445706,0.00007933113,0.011912223,0.00061763125,0.00022547241,0.006958925],"study_design_scores_gemma":[0.0000030225397,0.000037723978,0.99841106,0.0000029704909,0.000007926749,0.0000871637,0.00030364597,0.00014691528,0.00040232428,0.0002049204,0.0003896134,0.000002716958],"about_ca_topic_score_codex":0.00286256,"about_ca_topic_score_gemma":0.0022509806,"teacher_disagreement_score":0.0031545444,"about_ca_system_score_codex":0.00028443063,"about_ca_system_score_gemma":0.00016844222,"threshold_uncertainty_score":0.010553002},"labels":[],"label_agreement":null},{"id":"W2026371921","doi":"10.1086/588651","title":"Measuring Column Densities in Quasar Outflows: VLT Observations of QSO 2359−1241","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Outflow; Quasar; Absorption (acoustics); Column (typography); Resolution (logic); Spectral line; Scale (ratio); Resonance (particle physics)","score_opus":0.03447703730115367,"score_gpt":0.212489347932753,"score_spread":0.17801231063159934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026371921","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978668,0.00007134343,0.000893766,0.0000142299,0.0000023411867,0.00000314694,0.00050809915,0.000057601264,0.00058260444],"genre_scores_gemma":[0.99873286,0.000031466883,0.0005586001,0.0000066308394,0.0000066345524,0.0000023577982,0.00059659354,0.0000053569534,0.000059441325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999119,0.000010215266,0.0000044931207,0.000027495815,0.000024728315,0.000021119726],"domain_scores_gemma":[0.99974805,0.000055123142,0.00008475287,0.000019303521,0.00002710715,0.0000656772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020074962,0.00021149781,0.00023761805,0.0009742638,0.00027626823,0.00047656064,0.00025985524,0.0001965127,0.00076917344],"category_scores_gemma":[0.00067032943,0.00014367081,0.00020784345,0.00059180113,0.00021527633,0.00026882094,0.00029510426,0.00019206078,0.00015961699],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022316442,0.0001384909,0.8279156,0.00009473856,0.00015772475,0.00041014148,0.00047346248,0.012531308,0.13501637,0.0015455413,0.0007722034,0.020721367],"study_design_scores_gemma":[0.000013714155,0.000069144655,0.9700402,0.000007739954,0.000031783842,0.0002167876,0.000111771726,0.02252179,0.0057300413,0.0004885428,0.00074950414,0.000018934976],"about_ca_topic_score_codex":0.004370342,"about_ca_topic_score_gemma":0.0051847645,"teacher_disagreement_score":0.004370342,"about_ca_system_score_codex":0.0004183095,"about_ca_system_score_gemma":0.00009219403,"threshold_uncertainty_score":0.008689761},"labels":[],"label_agreement":null},{"id":"W2026401307","doi":"10.1086/338358","title":"The Structure of the Magnetic Field in the Outer Galaxy from Rotation Measure Observations through the Disk","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Galaxy; Polarization (electrochemistry); Magnetic field; Astronomy; Galactic plane; Rotation (mathematics); Geometry","score_opus":0.013163336911836652,"score_gpt":0.2213475499347557,"score_spread":0.20818421302291903,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026401307","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99461836,0.0006207664,0.0005095488,0.000039393755,0.0000023317523,0.000005960297,0.0011162761,0.000021811948,0.0030655263],"genre_scores_gemma":[0.9965648,0.0005263872,0.000592442,0.000010177966,0.000008113537,0.0000020417835,0.001943243,0.000005992729,0.00034693215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999409,0.0000056024096,0.0000031040843,0.000015204474,0.000019667648,0.000015539854],"domain_scores_gemma":[0.9996879,0.000043984182,0.000086563465,0.000024480603,0.00009764917,0.000059522743],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009329572,0.00014341636,0.00011465861,0.0018766097,0.00024082923,0.00092802977,0.0002527548,0.0001449316,0.00080442196],"category_scores_gemma":[0.00092151354,0.00014961867,0.00009574075,0.0017519839,0.00029467884,0.00027416568,0.00031552534,0.0001521811,0.0003303552],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014074506,0.000019650313,0.91127527,0.00009955261,0.000042453386,0.00022875221,0.00066994823,0.0011815826,0.028520653,0.0007492861,0.00061380136,0.05645829],"study_design_scores_gemma":[0.0000020320504,0.0000068185464,0.998447,0.0000066573048,0.00000986863,0.000072981704,0.000055746885,0.00036394532,0.00032871208,0.000099743505,0.00060397654,0.000002652883],"about_ca_topic_score_codex":0.1007329,"about_ca_topic_score_gemma":0.1739519,"teacher_disagreement_score":0.1007329,"about_ca_system_score_codex":0.00078151235,"about_ca_system_score_gemma":0.0004535872,"threshold_uncertainty_score":0.20029312},"labels":[],"label_agreement":null},{"id":"W2026436661","doi":"10.1086/321647","title":"SN 1993J VLBI. I. The Center of the Explosion and a Limit on Anisotropic Expansion","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Very-long-baseline interferometry; Astrophysics; Proper motion; Shell (structure); Shock (circulatory); Supernova; Isotropy; Rotation (mathematics); Anisotropy; Geometry; Optics","score_opus":0.01366350417279719,"score_gpt":0.22134955511318358,"score_spread":0.2076860509403864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026436661","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9290429,0.0021903715,0.014712171,0.0003186318,0.000043802833,0.0000614089,0.008496954,0.0005396199,0.0445942],"genre_scores_gemma":[0.9731463,0.0006527836,0.009335825,0.00011327407,0.00004084674,0.000052447653,0.013280512,0.000118115764,0.0032598318],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997272,0.000034623194,0.000019701567,0.00007598149,0.00007829022,0.00006426585],"domain_scores_gemma":[0.99946564,0.00006091574,0.00021111418,0.00008619144,0.00012129454,0.000054814154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050173735,0.00033508617,0.0002693163,0.0007128535,0.00047194393,0.001133537,0.00034156424,0.00027882334,0.0017670661],"category_scores_gemma":[0.0018260829,0.00030970213,0.00015108343,0.00061018683,0.00016834588,0.00035206886,0.0004722344,0.00031617272,0.0010265925],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002085568,0.00009364438,0.80759555,0.00021985424,0.00018002909,0.0007837272,0.00020672154,0.010840409,0.06548523,0.03368256,0.010669449,0.068157315],"study_design_scores_gemma":[0.000046518173,0.00005414926,0.92861074,0.00004845278,0.00007319592,0.0015434768,0.00007406262,0.029235318,0.008978139,0.007553224,0.023758626,0.000024157995],"about_ca_topic_score_codex":0.024214555,"about_ca_topic_score_gemma":0.044021066,"teacher_disagreement_score":0.024214555,"about_ca_system_score_codex":0.0011070363,"about_ca_system_score_gemma":0.0003473852,"threshold_uncertainty_score":0.04814726},"labels":[],"label_agreement":null},{"id":"W2026447544","doi":"10.1088/0004-637x/759/1/62","title":"RELATIONSHIP BETWEEN LOW AND HIGH FREQUENCIES IN δ SCUTI STARS: PHOTOMETRIC<i>KEPLER</i>AND SPECTROSCOPIC ANALYSES OF THE RAPID ROTATOR KIC 8054146","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Amplitude; Astrophysics; Low frequency; Stars; Equidistant; Rotation (mathematics); Frequency domain; Asteroseismology; Optics; Astronomy; Geometry; Mathematics","score_opus":0.035852623328280125,"score_gpt":0.2770356637144285,"score_spread":0.24118304038614838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026447544","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99855715,0.00011450335,0.00022675298,0.0000125152355,0.0000027687054,0.0000038551857,0.00016666035,0.000016647457,0.00089922897],"genre_scores_gemma":[0.9989298,0.00003434132,0.0003141478,0.00001013423,0.000006900019,0.000006964251,0.00044327698,0.000009395891,0.00024493216],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981934,0.000012604021,0.000021320006,0.00006524451,0.00004398476,0.000037523838],"domain_scores_gemma":[0.9992113,0.00013703154,0.00029481985,0.000067896886,0.00014390986,0.00014502404],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021769029,0.0002450188,0.00022514634,0.0024824527,0.0004995191,0.0006789982,0.00033890287,0.00042836196,0.0007633119],"category_scores_gemma":[0.0009868278,0.00025254788,0.00018956499,0.0010750783,0.00044865743,0.0003030667,0.0005404714,0.00046175902,0.00035201886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022687511,0.0000703699,0.91272885,0.00004546682,0.00005197408,0.00020057132,0.0003389863,0.00029477323,0.07503151,0.0001127749,0.00012442691,0.010773317],"study_design_scores_gemma":[0.00000367884,0.000023102804,0.99818367,0.0000027746255,0.000006378083,0.00009305921,0.00004757362,0.000165464,0.0012675929,0.000027716782,0.0001756911,0.0000033140407],"about_ca_topic_score_codex":0.0028439888,"about_ca_topic_score_gemma":0.0048409766,"teacher_disagreement_score":0.0028439888,"about_ca_system_score_codex":0.00038846806,"about_ca_system_score_gemma":0.00015172614,"threshold_uncertainty_score":0.0056548715},"labels":[],"label_agreement":null},{"id":"W2026578750","doi":"10.1088/0004-637x/710/2/1395","title":"RADIATIVE HYDRODYNAMIC SIMULATIONS OF HD209458b: TEMPORAL VARIABILITY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Radiative transfer; Opacity; Decoupling (probability); Thermal; Radiant energy; Thermal radiation; Atmospheric models; Stellar atmosphere; Range (aeronautics); Computational astrophysics","score_opus":0.007149223504738102,"score_gpt":0.2331845616866182,"score_spread":0.2260353381818801,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026578750","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99250245,0.000070421775,0.0020013603,0.00021457173,0.000026126752,0.000018621695,0.0007992168,0.00020227398,0.004164962],"genre_scores_gemma":[0.99762493,0.000024801413,0.0013174897,0.00003443473,0.000010336816,0.000017881925,0.0006131183,0.000031589203,0.00032539884],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999027,0.00002041824,0.000004691647,0.00001687902,0.00002357625,0.00003174668],"domain_scores_gemma":[0.999759,0.000073650124,0.000036031674,0.000025231138,0.0000360633,0.000069953414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025698732,0.00034653692,0.00034326612,0.00032551808,0.0004145135,0.00049088104,0.0008281033,0.0007302601,0.001004137],"category_scores_gemma":[0.0008537869,0.00021525583,0.00047949352,0.0004467193,0.00050354336,0.00032085512,0.00059090497,0.0005300602,0.00013317697],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053478265,0.00036478258,0.035901126,0.00005234948,0.00014192278,0.000523381,0.00027084776,0.937237,0.012913846,0.004766768,0.0019992918,0.0052938564],"study_design_scores_gemma":[0.000075588265,0.000036912767,0.008986762,0.000003505026,0.000010541309,0.000028028566,0.00004478563,0.9890409,0.0008168945,0.0003988819,0.00054631167,0.000010850493],"about_ca_topic_score_codex":0.024335992,"about_ca_topic_score_gemma":0.012308598,"teacher_disagreement_score":0.024335992,"about_ca_system_score_codex":0.0010055462,"about_ca_system_score_gemma":0.00047613788,"threshold_uncertainty_score":0.04838866},"labels":[],"label_agreement":null},{"id":"W2026609384","doi":"10.1088/0004-637x/799/2/168","title":"STRONG LENS TIME DELAY CHALLENGE. I. EXPERIMENTAL DESIGN","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Set (abstract data type); Quasar; Computer science; Measure (data warehouse); Lens (geology); Through-the-lens metering; Large Synoptic Survey Telescope; Plug-in; Cosmology; Telescope; Data mining; Physics; Astrophysics; Galaxy; Optics","score_opus":0.028182919097933627,"score_gpt":0.2415958800852224,"score_spread":0.21341296098728876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026609384","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.18975484,0.0041792216,0.5630219,0.0047355294,0.0030647682,0.0554505,0.11692034,0.008859355,0.05401355],"genre_scores_gemma":[0.26255295,0.0016549461,0.4570462,0.0058353436,0.00087082287,0.1705636,0.08032219,0.0028294325,0.018324524],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9862487,0.0063003255,0.001097681,0.0030568321,0.0025970128,0.0006995527],"domain_scores_gemma":[0.95603305,0.018903978,0.004141632,0.012361224,0.006836728,0.0017233992],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.021672009,0.0017960507,0.0013141618,0.001021293,0.0024638239,0.0033761968,0.0040836553,0.0032943368,0.021373514],"category_scores_gemma":[0.062434696,0.0014321962,0.0021249764,0.0016723187,0.0027092488,0.0022408469,0.003652858,0.0039549903,0.00708903],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.032561116,0.010967953,0.08221087,0.012236249,0.0029839745,0.0010426672,0.0023133818,0.13955829,0.046969257,0.13379526,0.23060623,0.30475476],"study_design_scores_gemma":[0.00984295,0.015560828,0.057082728,0.0018141955,0.0016156269,0.0011487247,0.0015947209,0.16408375,0.05080855,0.2006522,0.49485642,0.00093934324],"about_ca_topic_score_codex":0.0040438888,"about_ca_topic_score_gemma":0.0040924363,"teacher_disagreement_score":0.021672009,"about_ca_system_score_codex":0.0023853169,"about_ca_system_score_gemma":0.0046185595,"threshold_uncertainty_score":0.11461389},"labels":[],"label_agreement":null},{"id":"W2026653462","doi":"10.1086/309393","title":"Binary Microlensing Events from the MACHO Project","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Gravitational microlensing; Physics; Caustic (mathematics); Bulge; Astrophysics; Gravitational lens; Binary number; Astronomy; Mass ratio; Binary star; Lens (geology); Stars; Galaxy; Optics","score_opus":0.012179041441134953,"score_gpt":0.23179405824992033,"score_spread":0.21961501680878537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026653462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91538996,0.0017848868,0.003036712,0.0010616039,0.00020200155,0.00018622962,0.02835112,0.0014133973,0.048574083],"genre_scores_gemma":[0.9237,0.00036793278,0.005971213,0.00025574435,0.00023531151,0.000072612806,0.061424047,0.00034946992,0.007623709],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993155,0.000072330986,0.000024866338,0.0001078623,0.00033132263,0.00014810813],"domain_scores_gemma":[0.9991658,0.00010594677,0.00016378447,0.00018670413,0.00015457842,0.0002232462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006012494,0.00034873988,0.0003508322,0.0015385718,0.00082291785,0.0014606745,0.0004140524,0.00055298756,0.002734988],"category_scores_gemma":[0.0016393189,0.00015503542,0.00022747672,0.0012978165,0.00021032362,0.0005736445,0.002344166,0.00054599124,0.0010334408],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0033004512,0.00089710177,0.46640897,0.0005758203,0.00038564697,0.0049302783,0.003385257,0.002713543,0.021422647,0.01775292,0.19858356,0.2796438],"study_design_scores_gemma":[0.0001767205,0.00013084972,0.8412469,0.00007678962,0.00008351922,0.0019086414,0.0012676301,0.0101334425,0.004078449,0.004959377,0.13587867,0.00005894946],"about_ca_topic_score_codex":0.0070798807,"about_ca_topic_score_gemma":0.014393006,"teacher_disagreement_score":0.0070798807,"about_ca_system_score_codex":0.00055691553,"about_ca_system_score_gemma":0.00033809157,"threshold_uncertainty_score":0.014077306},"labels":[],"label_agreement":null},{"id":"W2026673350","doi":"10.1088/0004-637x/782/2/74","title":"CONSTRAINTS ON COSMOLOGY FROM THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM OF THE 2500 deg<sup>2</sup>SPT-SZ SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":276,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; National Energy Research Scientific Computing Center; U.S. Department of Energy; McGill University; Gordon and Betty Moore Foundation; Office of Science; Canada Research Chairs; National Aeronautics and Space Administration; National Science Foundation","keywords":"Cosmic microwave background; Physics; Astrophysics; Neutrino; Spectral density; Cosmology; Context (archaeology); Spectral index; Baryon acoustic oscillations; Lambda; Degenerate energy levels; Inflation (cosmology); Particle physics; Dark energy; Theoretical physics; Spectral line; Quantum mechanics; Statistics","score_opus":0.011892034596873742,"score_gpt":0.2368913471014666,"score_spread":0.22499931250459285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026673350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.992305,0.00020198913,0.0020144528,0.00015659606,0.000008405449,0.000005195345,0.0014602714,0.000060525006,0.003787578],"genre_scores_gemma":[0.9951794,0.00013292962,0.0011422082,0.000050592294,0.000025288633,0.000007267979,0.0032520182,0.000028343567,0.00018201393],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954224,0.00015410165,0.000024516517,0.00008991054,0.00012192701,0.000067302135],"domain_scores_gemma":[0.99678683,0.0010884135,0.000803628,0.00060094555,0.00029171645,0.00042846877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001769037,0.0006468885,0.0003655076,0.00088449847,0.0002744476,0.0013244464,0.0006010769,0.0002859977,0.0027426798],"category_scores_gemma":[0.0039874194,0.0002075666,0.0005664128,0.00148966,0.0006158084,0.0007450674,0.00089438894,0.00042962338,0.00058005],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009409812,0.000040754025,0.94618976,0.00011034387,0.00029562798,0.00053421815,0.00027482284,0.012907705,0.011594876,0.008426454,0.0018724767,0.016811943],"study_design_scores_gemma":[0.00003145443,0.00006372759,0.9766483,0.00003835823,0.00008179803,0.00024153235,0.00017789366,0.014453622,0.0015885162,0.002749702,0.0039023606,0.000022774164],"about_ca_topic_score_codex":0.0034077032,"about_ca_topic_score_gemma":0.004045715,"teacher_disagreement_score":0.0034077032,"about_ca_system_score_codex":0.00027817255,"about_ca_system_score_gemma":0.00023799375,"threshold_uncertainty_score":0.009355664},"labels":[],"label_agreement":null},{"id":"W2026721335","doi":"10.1086/322515","title":"<i>Chandra</i>X‐Ray Observations of G11.2−0.3: Implications for Pulsar Ages","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Pulsar wind nebula; Millisecond pulsar; Supernova remnant; Astronomy; X-ray pulsar; Pulsar planet; RADIUS; Nebula; Binary pulsar; Observatory; Supernova; Stars","score_opus":0.038864591698688694,"score_gpt":0.3485172740085384,"score_spread":0.30965268230984966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026721335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9855397,0.003468727,0.0022925944,0.0011964004,0.00007709973,0.000013288919,0.0018331566,0.00030173876,0.0052773394],"genre_scores_gemma":[0.99463755,0.0010121401,0.002103817,0.00029859573,0.000086169865,0.0000064273972,0.0012144791,0.00004350855,0.00059728854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999256,0.0000067476008,0.0000064710716,0.000020843603,0.000013101614,0.000027290465],"domain_scores_gemma":[0.9992887,0.00016180378,0.00031061657,0.00007908913,0.0000580984,0.00010173295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029478254,0.0002633046,0.00018136413,0.00095390016,0.00041100426,0.0013669183,0.0003810619,0.000410978,0.0013622975],"category_scores_gemma":[0.0009100556,0.00019129063,0.00019111161,0.0008905983,0.00043209468,0.00051263475,0.0004963436,0.00038409667,0.0003782818],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009717377,0.00007525916,0.8508915,0.0003468888,0.00009453829,0.0015465381,0.00062800024,0.0029645187,0.07993328,0.004832978,0.007818904,0.049895875],"study_design_scores_gemma":[0.000017419039,0.000043544795,0.98568404,0.00003062196,0.000039578517,0.0010838729,0.00014554437,0.0008321084,0.0049026976,0.0019009785,0.0052882065,0.000031369258],"about_ca_topic_score_codex":0.002991466,"about_ca_topic_score_gemma":0.004383444,"teacher_disagreement_score":0.002991466,"about_ca_system_score_codex":0.0004373588,"about_ca_system_score_gemma":0.00011442008,"threshold_uncertainty_score":0.0059481263},"labels":[],"label_agreement":null},{"id":"W2026772322","doi":"10.1086/507125","title":"<i>Chandra</i>and<i>XMM‐Newton</i>Observations of the Vela‐like Pulsar B1046−58","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Pulsar; Pulsar wind nebula; Luminosity; Outflow; Supernova remnant; Equipartition theorem; Nebula","score_opus":0.011438708666693782,"score_gpt":0.26923408490732875,"score_spread":0.257795376240635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026772322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9611085,0.0030762742,0.002864451,0.00055089896,0.00014899827,0.00009741129,0.011662287,0.0012565646,0.019234618],"genre_scores_gemma":[0.9652497,0.0019152422,0.014811295,0.00053800904,0.00032841763,0.00009039998,0.014715245,0.00020200716,0.0021496485],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998468,0.000010622985,0.000011277006,0.000029708517,0.000051760173,0.00004974747],"domain_scores_gemma":[0.9994123,0.000069610694,0.00023229096,0.000085313055,0.00006042832,0.00014005724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023452324,0.0003548488,0.00028858913,0.0036646172,0.0006597435,0.0008198894,0.00059471204,0.0003742374,0.0023358914],"category_scores_gemma":[0.00054600916,0.00029542515,0.00041094277,0.0015218467,0.0002756171,0.00044421753,0.0006878115,0.00062175596,0.0005655527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014151939,0.0006951361,0.52892405,0.0012560685,0.00083949236,0.0036532716,0.0009023142,0.0040668687,0.28380767,0.0025784974,0.03562088,0.13624072],"study_design_scores_gemma":[0.000046441546,0.00011997718,0.9746119,0.00008392452,0.00008962229,0.002443431,0.00010293244,0.0010868583,0.008150788,0.00037694396,0.012837018,0.000050139864],"about_ca_topic_score_codex":0.0030962375,"about_ca_topic_score_gemma":0.007553855,"teacher_disagreement_score":0.0036646172,"about_ca_system_score_codex":0.00032470442,"about_ca_system_score_gemma":0.00018183234,"threshold_uncertainty_score":0.007814407},"labels":[],"label_agreement":null},{"id":"W2026784455","doi":"10.1088/0004-637x/767/1/71","title":"MULTI-WAVELENGTH OBSERVATIONS OF SUPERNOVA 2011ei: TIME-DEPENDENT CLASSIFICATION OF TYPE IIb AND Ib SUPERNOVAE AND IMPLICATIONS FOR THEIR PROGENITORS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Supernova; Astrophysics; Physics; Balmer series; Star (game theory); Light curve; Solar mass; Type (biology); Astronomy; Wavelength; Spectral line; Galaxy; Emission spectrum; Optics; Geology","score_opus":0.039111170681149485,"score_gpt":0.2563049336091916,"score_spread":0.2171937629280421,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026784455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99648607,0.00038728444,0.00035072904,0.000051870742,0.000012194764,0.0000083864,0.0008817605,0.00001754071,0.0018041749],"genre_scores_gemma":[0.9966444,0.000253459,0.0006943185,0.00003570667,0.000020690304,0.000011546559,0.0014616486,0.000013783095,0.00086462375],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998221,0.000018042858,0.000019920833,0.000062211926,0.000034726916,0.000043084106],"domain_scores_gemma":[0.99887043,0.00010785386,0.0004358843,0.00009805897,0.00017215825,0.00031546268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005348993,0.00018587257,0.0001792536,0.0022784437,0.0003889802,0.0008066192,0.0002895686,0.00033065767,0.0014124044],"category_scores_gemma":[0.0009400952,0.0002146279,0.00019616992,0.001361516,0.0002159346,0.00044108534,0.00081064645,0.0003379957,0.00035044563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002970434,0.000068122456,0.9494288,0.00002742586,0.00005418552,0.000097500546,0.00021345975,0.00011324746,0.037354197,0.0002528135,0.00033364492,0.011759477],"study_design_scores_gemma":[0.0000019426934,0.000011982972,0.99878556,0.000003780547,0.000007864165,0.00014341938,0.00007337227,0.0001066086,0.00044446037,0.000049762722,0.0003683968,0.000002900156],"about_ca_topic_score_codex":0.0038365652,"about_ca_topic_score_gemma":0.010857243,"teacher_disagreement_score":0.0038365652,"about_ca_system_score_codex":0.00034262662,"about_ca_system_score_gemma":0.00021712833,"threshold_uncertainty_score":0.0076285005},"labels":[],"label_agreement":null},{"id":"W2026888296","doi":"10.1088/0004-637x/798/1/65","title":"ERRATUM: “THE SPITZER SURVEY OF INTERSTELLAR CLOUDS IN THE GOULD BELT. VI. THE AURIGA–CALIFORNIA MOLECULAR CLOUD OBSERVED WITH IRAC AND MIPS” (2014, ApJ, 786, 37)","year":2014,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Law, logistics, and international trade","field":"Business, Management and Accounting","cited_by":1,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Molecular cloud; Interstellar cloud; Astrobiology; Astrophysics; Astronomy; Stars","score_opus":0.028100364782395935,"score_gpt":0.2268490208068612,"score_spread":0.19874865602446526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026888296","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00065270514,0.0012071437,0.00033485226,0.04935245,0.9282702,0.000037383088,0.004804911,0.00045161537,0.014888747],"genre_scores_gemma":[0.015822582,0.008537206,0.0038287565,0.08453213,0.18119907,0.00017966912,0.021079449,0.0019537152,0.68286747],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99792695,0.00016718153,0.00044819617,0.0002230615,0.0010633179,0.00017120424],"domain_scores_gemma":[0.99094605,0.0011612875,0.00062127714,0.00055428484,0.0062831226,0.00043408733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013345903,0.0016734559,0.0013199082,0.0040902467,0.004084224,0.0029191915,0.0024112104,0.0036261138,0.05216445],"category_scores_gemma":[0.01730813,0.0009244551,0.001070667,0.0028724545,0.0013289637,0.0023850594,0.0017539387,0.0058131986,0.036506],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000016061622,0.000007274108,0.000103542865,0.00004000985,0.0000035509474,0.00011125459,0.000015880873,0.00002412943,0.00003271437,0.00035617416,0.99653363,0.0027557095],"study_design_scores_gemma":[0.000018364166,0.00001773792,0.0022095144,0.00021215637,0.000019854013,0.00022203432,0.00011478721,0.000087746164,0.00028178724,0.00064786035,0.9961396,0.000028396415],"about_ca_topic_score_codex":0.053997073,"about_ca_topic_score_gemma":0.06087436,"teacher_disagreement_score":0.053997073,"about_ca_system_score_codex":0.0034250892,"about_ca_system_score_gemma":0.0056676827,"threshold_uncertainty_score":0.1745075},"labels":[],"label_agreement":null},{"id":"W2026992861","doi":"10.1088/0004-637x/744/1/26","title":"LATE-TIME LIGHT CURVES OF TYPE II SUPERNOVAE: PHYSICAL PROPERTIES OF SUPERNOVAE AND THEIR ENVIRONMENT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Light curve; Supernova; Physics; Photometry (optics); Astrophysics; Flattening; Astronomy; Stars","score_opus":0.016819671111733756,"score_gpt":0.19428638977159696,"score_spread":0.1774667186598632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2026992861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977623,0.00014266463,0.00033337713,0.000006989214,0.0000021288188,0.000003308386,0.0008527945,0.000028886365,0.00086750346],"genre_scores_gemma":[0.99733114,0.00008165472,0.00030946254,0.000007130319,0.000006913275,0.000003293115,0.001870603,0.00000972842,0.0003800781],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991906,0.0000068807253,0.000009527503,0.00002267505,0.00001925262,0.00002250462],"domain_scores_gemma":[0.99923444,0.00010247133,0.00030509254,0.00004429984,0.00010286689,0.00021086112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018716193,0.00022158325,0.00015173903,0.0012832547,0.00014464305,0.00047250028,0.00014762758,0.00022419929,0.000991725],"category_scores_gemma":[0.00054852996,0.00008360463,0.00017117236,0.00066953554,0.00015083785,0.00026400416,0.00020882493,0.00021003402,0.00029088932],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010253265,0.000041339397,0.97810674,0.000018463366,0.000031519136,0.00010725815,0.00010216428,0.0004786725,0.015912306,0.00008582362,0.00018159437,0.004831582],"study_design_scores_gemma":[5.259047e-7,0.000016759079,0.9990127,9.450372e-7,0.000002428604,0.00008975251,0.000020614058,0.00020567057,0.0004781499,0.000015704798,0.00015507103,0.000001634015],"about_ca_topic_score_codex":0.0026708178,"about_ca_topic_score_gemma":0.0046669785,"teacher_disagreement_score":0.0026708178,"about_ca_system_score_codex":0.00018493264,"about_ca_system_score_gemma":0.00006719828,"threshold_uncertainty_score":0.0053105354},"labels":[],"label_agreement":null},{"id":"W2027045695","doi":"10.1088/0004-637x/707/1/738","title":"DAMPED LYα ABSORBER KINEMATICS AND OUTFLOWS FROM STARBURST GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Star formation; Galaxy; Interstellar medium; Velocity dispersion; Thermal; Meteorology","score_opus":0.007410642927050867,"score_gpt":0.2117920174780351,"score_spread":0.20438137455098424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027045695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987662,0.000034106684,0.0005834002,0.000026886217,0.0000025879374,0.0000042284782,0.00010351932,0.00003297465,0.0004461043],"genre_scores_gemma":[0.9988721,0.00002258274,0.0006890652,0.000008368805,0.0000025779145,0.000004852268,0.00018152034,0.000010395191,0.00020852196],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99987924,0.000025492307,0.000007785932,0.000032271335,0.000019163177,0.000035993893],"domain_scores_gemma":[0.99897826,0.00039494075,0.0002459222,0.000085643245,0.00007865469,0.00021671409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003398562,0.00044844297,0.0003239679,0.0004769819,0.0005908309,0.0011338758,0.00078064523,0.0007084612,0.0012578215],"category_scores_gemma":[0.002278462,0.0004495933,0.00051594415,0.00045577055,0.00069645466,0.0006637966,0.00067095866,0.0005381682,0.00012168511],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028109257,0.00021134694,0.12550426,0.00004584707,0.000080510246,0.00047112114,0.00025980207,0.8629866,0.0054276134,0.0020680432,0.0002867837,0.0023770204],"study_design_scores_gemma":[0.00007307774,0.0000826317,0.03242521,0.000007300547,0.000019997386,0.000073980205,0.00009778519,0.9652844,0.0010034372,0.0007798372,0.00013841267,0.00001397132],"about_ca_topic_score_codex":0.020184131,"about_ca_topic_score_gemma":0.0131928595,"teacher_disagreement_score":0.020184131,"about_ca_system_score_codex":0.0012031874,"about_ca_system_score_gemma":0.0004242751,"threshold_uncertainty_score":0.040133297},"labels":[],"label_agreement":null},{"id":"W2027055131","doi":"10.1088/0004-637x/696/1/567","title":"DISPERSION OF MAGNETIC FIELDS IN MOLECULAR CLOUDS. I","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":286,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Molecular cloud; Turbulence; Physics; Magnetic field; Dispersion (optics); Scale (ratio); Field (mathematics); Computational physics; Statistical physics; Astrophysics; Mechanics; Optics; Mathematics; Quantum mechanics; Stars","score_opus":0.005014730283440883,"score_gpt":0.2212507498824231,"score_spread":0.21623601959898223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027055131","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.16150416,0.0032553715,0.81606,0.00031332514,0.00035751998,0.00007699363,0.0009050977,0.0013823742,0.016145192],"genre_scores_gemma":[0.75446075,0.001103823,0.23599967,0.00007702116,0.00022727791,0.000039619998,0.00061584,0.00021034067,0.007265593],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99984086,0.000016652048,0.000008297555,0.000032872784,0.0000828554,0.000018367195],"domain_scores_gemma":[0.9995974,0.00010111158,0.000106461164,0.000076021846,0.00008808098,0.000031072806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031852053,0.00025489533,0.00018767589,0.0014591869,0.0006197545,0.00070817966,0.0006482781,0.0003247218,0.0013036025],"category_scores_gemma":[0.0019605388,0.00020513203,0.00020012562,0.0008808337,0.00039332878,0.00079535955,0.00063351507,0.00053889194,0.00057465443],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029665173,0.00008862523,0.08541962,0.00036542938,0.00013165537,0.0005100983,0.0011153821,0.11467013,0.1325361,0.16073692,0.008047225,0.4960822],"study_design_scores_gemma":[0.000063514985,0.00012392548,0.052257217,0.00012701804,0.000063942425,0.0011070404,0.00023177137,0.75558615,0.06826975,0.074227095,0.04781003,0.00013247295],"about_ca_topic_score_codex":0.0058523957,"about_ca_topic_score_gemma":0.004934692,"teacher_disagreement_score":0.0058523957,"about_ca_system_score_codex":0.0005495093,"about_ca_system_score_gemma":0.00034298826,"threshold_uncertainty_score":0.011636674},"labels":[],"label_agreement":null},{"id":"W2027089662","doi":"10.1088/0004-637x/778/2/103","title":"THE ACS LCID PROJECT. IX. IMPRINTS OF THE EARLY UNIVERSE IN THE RADIAL VARIATION OF THE STAR FORMATION HISTORY OF DWARF GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Astronomy; Elliptical galaxy; Dwarf spheroidal galaxy; Local Group; Galaxy; Lenticular galaxy; Population; Galaxy group","score_opus":0.007956457127173916,"score_gpt":0.18882264430928328,"score_spread":0.18086618718210937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027089662","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0031182151,0.0007237483,0.0022455622,0.001005648,0.00040820052,0.00015975791,0.9319958,0.023771998,0.03657103],"genre_scores_gemma":[0.01206415,0.0006468103,0.010116228,0.0005097602,0.0003641373,0.00041672727,0.9560172,0.005393292,0.014471748],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99906284,0.00006118994,0.000039882492,0.00016685849,0.0005159989,0.0001531317],"domain_scores_gemma":[0.9981718,0.00016025448,0.00019784259,0.0004996897,0.00047118263,0.0004991558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00182868,0.0013861946,0.0020131108,0.0052896324,0.0014578827,0.005466985,0.0034187606,0.0011636557,0.13891523],"category_scores_gemma":[0.0024787206,0.0007913893,0.0012069506,0.007365812,0.0003143852,0.0019449317,0.0037684003,0.0016088615,0.099849574],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001833478,0.00006877654,0.0034890226,0.0002432369,0.00006816217,0.00007471008,0.00007804485,0.00026908494,0.000996666,0.0019622794,0.9695905,0.022976141],"study_design_scores_gemma":[0.00045463542,0.000025748694,0.030757222,0.0001821785,0.00007951377,0.00010733238,0.000093844465,0.0035107639,0.0016689245,0.004780427,0.95828,0.00005951939],"about_ca_topic_score_codex":0.034451082,"about_ca_topic_score_gemma":0.056844037,"teacher_disagreement_score":0.13891523,"about_ca_system_score_codex":0.0017443508,"about_ca_system_score_gemma":0.0019255604,"threshold_uncertainty_score":0.46471775},"labels":[],"label_agreement":null},{"id":"W2027099564","doi":"10.1086/504316","title":"Modeling Tidal Streams in Evolving Dark Matter Halos","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Galaxy; Dark matter; Astronomy; Dark matter halo; Galaxy formation and evolution; Milky Way; Gravitational potential; Halo","score_opus":0.005644215049241696,"score_gpt":0.1988766682549961,"score_spread":0.19323245320575438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027099564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99228597,0.00009106221,0.006070913,0.00010025388,0.000008080812,0.000015625345,0.00015354276,0.00007835543,0.0011962182],"genre_scores_gemma":[0.99701023,0.00010047789,0.0020796277,0.000021689846,0.000008064918,0.000015363925,0.00012173302,0.000024720552,0.0006180176],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990475,0.000032668675,0.0000054550906,0.000015913245,0.000011376879,0.000029875258],"domain_scores_gemma":[0.9989768,0.00048041643,0.00018407105,0.00007169658,0.00009107495,0.00019589628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006619977,0.00041940415,0.0004724012,0.00084478,0.0005180743,0.0009391963,0.00095060904,0.0008102244,0.0010410586],"category_scores_gemma":[0.0029693437,0.00050003786,0.0005229553,0.0005797838,0.0009052675,0.0010870198,0.0009762778,0.00041898337,0.00017417608],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000080618665,0.000027608365,0.0142403105,0.000013006415,0.00003205138,0.00009447189,0.000087514236,0.98032445,0.00065677695,0.0032269894,0.000096780226,0.0011194326],"study_design_scores_gemma":[0.000028662604,0.0000146655,0.0009929441,0.000002923471,0.0000069905195,0.0000068975105,0.000023832397,0.99748343,0.00013027438,0.0011782871,0.00012579234,0.000005385991],"about_ca_topic_score_codex":0.035930716,"about_ca_topic_score_gemma":0.02000183,"teacher_disagreement_score":0.035930716,"about_ca_system_score_codex":0.0012026128,"about_ca_system_score_gemma":0.00076667365,"threshold_uncertainty_score":0.07144314},"labels":[],"label_agreement":null},{"id":"W2027199817","doi":"10.1088/0004-637x/734/2/100","title":"SELF-SIMILAR SOLUTIONS OF TRIAXIAL DARK MATTER HALOS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Halo; Dark matter; Physics; Gravitational collapse; Adiabatic process; Structure formation; Gravitation; Classical mechanics; Simple (philosophy); Statistical physics; Dark matter halo; Astrophysics; Theoretical physics; Galaxy; Quantum mechanics","score_opus":0.014815400888954066,"score_gpt":0.2059100191390013,"score_spread":0.19109461825004725,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027199817","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9618719,0.00021261096,0.029190935,0.0003782583,0.000019719573,0.00004123983,0.00010853339,0.00010245469,0.0080743665],"genre_scores_gemma":[0.9930906,0.00013682681,0.003691315,0.00009319786,0.000023625269,0.00003377312,0.00011689731,0.000034833367,0.0027787588],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998367,0.000038580452,0.000007831146,0.000017986737,0.00003464915,0.00006415292],"domain_scores_gemma":[0.99934393,0.00010449568,0.00017561289,0.00004603463,0.000110968365,0.00021898752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048312597,0.00050822843,0.00047450222,0.0010831201,0.0006312597,0.0010420082,0.0007705395,0.00095385837,0.0018834262],"category_scores_gemma":[0.0023253362,0.0004099669,0.0007394088,0.0004721475,0.0014180979,0.0008691732,0.0019298439,0.00051573786,0.00018482668],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016913988,0.00011369591,0.008951634,0.00007229116,0.0001322209,0.0015549944,0.00070898875,0.8134243,0.016118614,0.15474355,0.0008090465,0.0032015776],"study_design_scores_gemma":[0.00007352315,0.00003261649,0.0026275085,0.000010518852,0.000009979422,0.00012093918,0.00016259206,0.96765566,0.0009010978,0.027988113,0.00039112646,0.000026325622],"about_ca_topic_score_codex":0.009792662,"about_ca_topic_score_gemma":0.003507233,"teacher_disagreement_score":0.009792662,"about_ca_system_score_codex":0.001045973,"about_ca_system_score_gemma":0.00067406846,"threshold_uncertainty_score":0.019471288},"labels":[],"label_agreement":null},{"id":"W2027215101","doi":"10.1088/0004-637x/765/2/89","title":"THE CIRCUMGALACTIC MEDIUM OF MASSIVE GALAXIES AT<i>z</i>∼ 3: A TEST FOR STELLAR FEEDBACK, GALACTIC OUTFLOWS, AND COLD STREAMS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":216,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Interstellar medium; Redshift; Virial theorem; Supernova; Accretion (finance); Spectral line; RADIUS; Quasar; Active galactic nucleus","score_opus":0.006326947103441335,"score_gpt":0.2008064666439247,"score_spread":0.19447951954048337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027215101","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989755,0.000039854178,0.00025606737,0.000019840536,0.0000017295893,0.0000025549534,0.00020423942,0.000045384262,0.00045482532],"genre_scores_gemma":[0.99883264,0.000028804861,0.00043337533,0.000012296837,0.000004103939,0.0000018336839,0.00056110567,0.00001690367,0.0001088958],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992776,0.000012501401,0.0000022426027,0.000020395359,0.000012385544,0.000024714325],"domain_scores_gemma":[0.99934596,0.00016727147,0.00012261639,0.00006150406,0.000026187205,0.00027649454],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027563996,0.00054948335,0.00026807308,0.00041438028,0.0002993097,0.0007001907,0.00043346328,0.00027001151,0.0011142514],"category_scores_gemma":[0.00065812294,0.00020158764,0.0006611875,0.00036458,0.00044092286,0.00041183515,0.0006736016,0.00045823248,0.00012093852],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001725885,0.00044903363,0.7964282,0.00008125545,0.00042391647,0.0007800932,0.0005229819,0.12583904,0.05616988,0.0050389306,0.0012761686,0.011264588],"study_design_scores_gemma":[0.00023810225,0.00037984093,0.7322972,0.000013488882,0.00014418362,0.00018555592,0.0003833599,0.25316262,0.0100417845,0.0019658606,0.0011487709,0.00003930177],"about_ca_topic_score_codex":0.02118068,"about_ca_topic_score_gemma":0.0110343555,"teacher_disagreement_score":0.02118068,"about_ca_system_score_codex":0.00051956257,"about_ca_system_score_gemma":0.00022095894,"threshold_uncertainty_score":0.042114794},"labels":[],"label_agreement":null},{"id":"W2027222648","doi":"10.1088/0004-637x/706/1/441","title":"<i>AKARI</i>INFRARED OBSERVATIONS OF THE SUPERNOVA REMNANT G292.0+1.8: UNVEILING CIRCUMSTELLAR MEDIUM AND SUPERNOVA EJECTA","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Ejecta; Supernova remnant; Supernova; Infrared; Shell (structure); Near-Earth supernova; Pulsar; Spectral line","score_opus":0.016447771112812655,"score_gpt":0.22434271588985058,"score_spread":0.20789494477703793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027222648","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99599874,0.00016899145,0.00051324326,0.000038333415,0.000009747647,0.00001116509,0.0008161418,0.000109451954,0.0023343263],"genre_scores_gemma":[0.9940812,0.00011657473,0.002216457,0.00005754309,0.000027304814,0.000010133313,0.00259704,0.00002806058,0.00086565985],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995315,0.0000033596584,0.000003278441,0.000010260935,0.000015567262,0.0000142333765],"domain_scores_gemma":[0.99985933,0.000010135528,0.000038221548,0.000018539913,0.000019563216,0.00005422279],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001316132,0.00025570858,0.0001638914,0.0010952522,0.00026910304,0.00033742035,0.0002532061,0.00023316921,0.0012756548],"category_scores_gemma":[0.00013767248,0.000113528455,0.00021784914,0.00048308616,0.00011518956,0.00017435869,0.00040539654,0.00027162916,0.0003399612],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012535463,0.00029373032,0.35860685,0.00012455901,0.00020403972,0.0019160804,0.0003589129,0.0018683159,0.61202997,0.00030422883,0.0036718885,0.019367794],"study_design_scores_gemma":[0.000015834441,0.00006622711,0.98829377,0.0000047475924,0.00003273887,0.00039278832,0.00006616373,0.00115612,0.008373959,0.000048462032,0.0015350854,0.000014048097],"about_ca_topic_score_codex":0.0032444503,"about_ca_topic_score_gemma":0.009115639,"teacher_disagreement_score":0.0032444503,"about_ca_system_score_codex":0.0001429279,"about_ca_system_score_gemma":0.00006295767,"threshold_uncertainty_score":0.00645113},"labels":[],"label_agreement":null},{"id":"W2027251073","doi":"10.1086/505902","title":"Keck Deep Fields. III. Luminosity‐dependent Evolution of the Ultraviolet Luminosity and Star Formation Rate Densities at<i>z</i>∼4, 3, and 2","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Luminosity; Galaxy; Redshift; Luminosity function; Reionization; Star formation; Astronomy; Galaxy formation and evolution; Context (archaeology)","score_opus":0.004099214111894172,"score_gpt":0.177328585552359,"score_spread":0.17322937144046482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027251073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93863237,0.00066209683,0.0030895018,0.00022291759,0.000022487677,0.00003847586,0.044914756,0.00037485608,0.012042539],"genre_scores_gemma":[0.95807326,0.00022820984,0.0041707885,0.00013911103,0.000020617816,0.00005829468,0.030466963,0.00008607479,0.0067566773],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987316,0.000010595299,0.0000050985327,0.000039246766,0.000024005556,0.000047904847],"domain_scores_gemma":[0.99914885,0.000100088815,0.00044058237,0.0001253268,0.00006799256,0.00011709137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042252179,0.00034015748,0.00019464918,0.0015275831,0.00028792841,0.0005927885,0.00033765478,0.00028317946,0.0031206773],"category_scores_gemma":[0.0008413683,0.00033502994,0.00030398407,0.0010255954,0.00024724254,0.00072240387,0.00054748397,0.00038316686,0.0013870193],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005022727,0.00012892074,0.9336038,0.00017376662,0.00016953959,0.00023217002,0.00031831936,0.004522212,0.010269225,0.0059529096,0.012063503,0.03206337],"study_design_scores_gemma":[0.000016389971,0.000027327496,0.9889549,0.000018820463,0.000020629588,0.00013724934,0.00006517656,0.0019961712,0.0021693727,0.0010464801,0.0055349325,0.000012524608],"about_ca_topic_score_codex":0.007987556,"about_ca_topic_score_gemma":0.011496548,"teacher_disagreement_score":0.007987556,"about_ca_system_score_codex":0.00063234597,"about_ca_system_score_gemma":0.00017751394,"threshold_uncertainty_score":0.015882134},"labels":[],"label_agreement":null},{"id":"W2027266897","doi":"10.1088/0004-637x/720/1/581","title":"SPECTROSCOPIC ANALYSIS OF HOT, HYDROGEN-RICH WHITE DWARFS: THE PRESENCE OF METALS AND THE BALMER-LINE PROBLEM","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; Université de Montréal","funders":"","keywords":"Balmer series; White dwarf; Physics; Astrophysics; Stars; Line (geometry); Spectral line; Stellar atmosphere; Atmosphere (unit); Helium; Astronomy; Emission spectrum; Atomic physics","score_opus":0.007968517035594948,"score_gpt":0.23235430134393514,"score_spread":0.2243857843083402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027266897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993112,0.000030010911,0.00035925672,0.0000046579544,8.246325e-7,0.0000014123259,0.00007343426,0.000010988947,0.00020818037],"genre_scores_gemma":[0.9990569,0.000023569588,0.00056042563,0.0000032921316,0.0000015158392,0.0000010558915,0.00024504578,0.00000396636,0.00010422027],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999268,0.000011010049,0.0000063034304,0.000023823155,0.000017182118,0.000014834657],"domain_scores_gemma":[0.9997142,0.000047267302,0.00007957048,0.000042887492,0.000038528113,0.00007747975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018994494,0.00024918714,0.000225592,0.00090976653,0.0003270326,0.00034594527,0.00021783107,0.00015718202,0.00030907444],"category_scores_gemma":[0.00048160428,0.000085911306,0.00022998975,0.00054068526,0.00021241006,0.00018532255,0.0002950024,0.0001013168,0.00012661141],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000839227,0.000027679045,0.9748472,0.00001536996,0.000042709562,0.00014470275,0.00017058314,0.0025577336,0.017415792,0.00019475115,0.00006269846,0.0044368547],"study_design_scores_gemma":[0.000007624842,0.000088948684,0.97932076,0.00000383278,0.00003651122,0.00029287286,0.000314163,0.014033619,0.005005593,0.0002697032,0.0006189151,0.000007516287],"about_ca_topic_score_codex":0.0050738277,"about_ca_topic_score_gemma":0.007994061,"teacher_disagreement_score":0.0050738277,"about_ca_system_score_codex":0.00024777162,"about_ca_system_score_gemma":0.0001328614,"threshold_uncertainty_score":0.010088563},"labels":[],"label_agreement":null},{"id":"W2027272595","doi":"10.1088/0004-637x/730/2/76","title":"COMMON ENVELOPE: ON THE MASS AND THE FATE OF THE REMNANT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Accretion (finance); Thermal; RADIUS; Phase (matter); Pulsar; Binary number; Mass transfer; Millisecond pulsar","score_opus":0.022265369882227326,"score_gpt":0.28340645490434996,"score_spread":0.26114108502212263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027272595","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9407727,0.013067738,0.016013179,0.0022909376,0.00011851187,0.000012956198,0.00008581006,0.000041860425,0.02759624],"genre_scores_gemma":[0.99460053,0.0018525032,0.0009365222,0.000102993916,0.000090866844,0.000004678894,0.00004747093,0.000023956954,0.0023405466],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99980956,0.00005409861,0.000011395493,0.00004958051,0.000035850655,0.000039451712],"domain_scores_gemma":[0.99922013,0.00021537463,0.00024386808,0.0001400804,0.00007983626,0.00010074623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011316846,0.00021147967,0.0002803093,0.00049362076,0.0007278024,0.0017174467,0.00065676705,0.00081962545,0.0020803579],"category_scores_gemma":[0.0034176495,0.0001261489,0.00021647058,0.00032720974,0.0025921983,0.0034897,0.0019595574,0.0006232888,0.00074454356],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014024671,0.00014173983,0.094151676,0.0003330705,0.00006721764,0.0030935907,0.002926715,0.00706725,0.025790486,0.6936592,0.0018594746,0.16950707],"study_design_scores_gemma":[0.00005860415,0.00086887594,0.124697685,0.00044113147,0.00008145184,0.005582711,0.0039044216,0.022061823,0.021105021,0.78697336,0.034119785,0.00010515029],"about_ca_topic_score_codex":0.0005796634,"about_ca_topic_score_gemma":0.00034266876,"teacher_disagreement_score":0.0020803579,"about_ca_system_score_codex":0.00061892986,"about_ca_system_score_gemma":0.0002460559,"threshold_uncertainty_score":0.0069594383},"labels":[],"label_agreement":null},{"id":"W2027305915","doi":"10.1088/0004-637x/774/2/140","title":"A STATISTICAL STUDY OF THE SPECTRAL HARDENING OF CONTINUUM EMISSION IN SOLAR FLARES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Bremsstrahlung; Solar flare; Astrophysics; Electron; Spectral line; Flare; Photon; Hardening (computing); Particle acceleration; Radiation; Spectral index; Magnetic reconnection; Plasma; Astronomy; Computational physics; Nuclear physics; Optics","score_opus":0.005330821721661713,"score_gpt":0.22388009505551815,"score_spread":0.21854927333385643,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027305915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99924433,0.000046704234,0.0003775804,0.000008991773,7.675987e-7,0.0000027560636,0.00011544736,0.0000088626075,0.00019462791],"genre_scores_gemma":[0.9995615,0.000030543506,0.000093507435,0.0000032562805,0.0000064248547,0.0000026030327,0.00025098815,0.0000024918932,0.000048779904],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99967563,0.00007925479,0.000031133677,0.00009631367,0.000067554,0.00005011042],"domain_scores_gemma":[0.9931467,0.003137183,0.002465387,0.0005518451,0.00036135502,0.00033747486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069182,0.00015565696,0.00019683733,0.0023395238,0.0002539038,0.0005059164,0.00020085818,0.00026177143,0.001033753],"category_scores_gemma":[0.0043871035,0.00011710277,0.0002742786,0.0013257123,0.00044686603,0.000372938,0.00030468154,0.0002098829,0.00017760537],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012121868,0.000023609498,0.99006337,0.000010146438,0.00008151948,0.0000979028,0.00008645628,0.00082101196,0.0032792236,0.00017012718,0.00006715824,0.0051782406],"study_design_scores_gemma":[0.0000015295811,0.00006415353,0.99692035,0.0000014918106,0.000017857197,0.00017479782,0.000067994035,0.0021590414,0.00036164207,0.00010708895,0.000119282835,0.0000047694793],"about_ca_topic_score_codex":0.0010703177,"about_ca_topic_score_gemma":0.00072106987,"teacher_disagreement_score":0.0023395238,"about_ca_system_score_codex":0.00014281455,"about_ca_system_score_gemma":0.0001279501,"threshold_uncertainty_score":0.003658712},"labels":[],"label_agreement":null},{"id":"W2027372417","doi":"10.1086/520799","title":"The Leo Elliptical NGC 3379: A Metal‐Poor Halo Emerges","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; McMaster University","funders":"","keywords":"Physics; Astrophysics; Metallicity; Galaxy; Elliptical galaxy; Astronomy; Stars; Halo; Dwarf galaxy; Galactic halo; Photometry (optics); Luminosity function; Luminosity","score_opus":0.00805160370552464,"score_gpt":0.2267529046537511,"score_spread":0.21870130094822646,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027372417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99815553,0.000044924527,0.00011903662,0.00003735996,9.1605574e-7,0.000002844025,0.0001273655,0.000010954226,0.001501021],"genre_scores_gemma":[0.99928206,0.000031870382,0.00020282803,0.0000116800975,0.000002515752,9.491475e-7,0.00020534931,0.0000040143177,0.00025888567],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999726,0.0000023433765,0.0000011126099,0.000007549465,0.000006887876,0.000009536867],"domain_scores_gemma":[0.99992,0.000009162361,0.000022412909,0.000011519103,0.000008348124,0.000028573746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006569991,0.00009921913,0.000086675434,0.00030326645,0.00025084193,0.000255247,0.000114774455,0.00008153589,0.0011171385],"category_scores_gemma":[0.00019915501,0.000072327006,0.000052348132,0.00024832974,0.00022359283,0.00016403805,0.00052394293,0.00010035316,0.00022155514],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031226897,0.000054005097,0.8707089,0.00004618041,0.000029187791,0.0015990693,0.00081749,0.00045874462,0.10627724,0.0019512279,0.0010140854,0.01673152],"study_design_scores_gemma":[0.000008864719,0.000037605612,0.9914492,0.000007506512,0.000009734355,0.00092712103,0.0003155973,0.00046826416,0.0022492867,0.0003449347,0.004177109,0.000004931471],"about_ca_topic_score_codex":0.0036172864,"about_ca_topic_score_gemma":0.006766373,"teacher_disagreement_score":0.0036172864,"about_ca_system_score_codex":0.00020745659,"about_ca_system_score_gemma":0.00007947284,"threshold_uncertainty_score":0.0071924925},"labels":[],"label_agreement":null},{"id":"W2027399712","doi":"10.1088/0004-637x/780/1/51","title":"THE EFFECTS OF IRRADIATION ON CLOUD EVOLUTION IN ACTIVE GALACTIC NUCLEI","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Opacity; Cloud computing; Active galactic nucleus; Photoionization; Focus (optics); Radiation pressure; Radiative transfer; Acceleration","score_opus":0.004965289878723089,"score_gpt":0.2086980159107308,"score_spread":0.20373272603200773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027399712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99406826,0.000530783,0.0025534506,0.00012905213,0.000021955177,0.000023518889,0.00012766765,0.000071840936,0.002473498],"genre_scores_gemma":[0.9981881,0.00027289032,0.0010097169,0.000033800912,0.000014642336,0.000008413047,0.00009596239,0.000046364745,0.00033006063],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999892,0.000027438113,0.0000051429165,0.0000149063235,0.000021300784,0.000039162],"domain_scores_gemma":[0.99912804,0.0004962936,0.00017823785,0.000039147235,0.00006882476,0.00008950045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028112292,0.0006863114,0.00048618237,0.00033089195,0.0005810617,0.0006285614,0.0007320571,0.00071228953,0.0009932877],"category_scores_gemma":[0.00203436,0.00026637982,0.0006320311,0.0004724422,0.00066891365,0.0004862028,0.00059433375,0.00063134934,0.000104554056],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032259882,0.00022026493,0.04434619,0.00013038362,0.00013361248,0.0008111174,0.00020141143,0.9093343,0.03636593,0.0029431407,0.00032717254,0.004863856],"study_design_scores_gemma":[0.000120196586,0.00034851374,0.027682114,0.000018714076,0.00006624524,0.00012566296,0.000094483585,0.95844,0.011230213,0.0011142074,0.0007238793,0.000035821216],"about_ca_topic_score_codex":0.014411626,"about_ca_topic_score_gemma":0.0053792996,"teacher_disagreement_score":0.014411626,"about_ca_system_score_codex":0.0010069568,"about_ca_system_score_gemma":0.00042863953,"threshold_uncertainty_score":0.02865547},"labels":[],"label_agreement":null},{"id":"W2027423464","doi":"10.1086/426132","title":"Globular Clusters with Dark Matter Halos. I. Initial Relaxation","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Dark matter; Velocity dispersion; Star cluster; Surface brightness; Cluster (spacecraft); Luminosity; Brightness","score_opus":0.005855742861077908,"score_gpt":0.21756507326051183,"score_spread":0.21170933039943393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027423464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98962104,0.0003757784,0.0051928386,0.00023509962,0.000026925643,0.00006115996,0.00034575388,0.00014275881,0.0039987178],"genre_scores_gemma":[0.9960861,0.00014002377,0.0022945793,0.00008089044,0.000014600276,0.000023623672,0.00028079405,0.00003777775,0.0010415363],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99978346,0.00006532796,0.000008721192,0.000038087368,0.000039717575,0.00006479998],"domain_scores_gemma":[0.9989735,0.00034138552,0.0001940141,0.00015452347,0.000088940214,0.00024769243],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005953617,0.0005205753,0.00045662528,0.00040308767,0.00075177185,0.00095271034,0.00076594495,0.0007889685,0.0020002984],"category_scores_gemma":[0.003149434,0.00039794573,0.00064822997,0.00042399325,0.00091159344,0.00085218775,0.0011448915,0.00075565436,0.00024998456],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047387322,0.00020772134,0.059681814,0.00014018583,0.00013034248,0.0007095765,0.00045799476,0.908881,0.0065818485,0.016164454,0.0013854714,0.005185749],"study_design_scores_gemma":[0.00027809545,0.0002132968,0.019047242,0.000022731876,0.00004241357,0.0002416301,0.0002959396,0.9590068,0.0038275192,0.014805584,0.0021752391,0.00004349277],"about_ca_topic_score_codex":0.014252394,"about_ca_topic_score_gemma":0.008628677,"teacher_disagreement_score":0.014252394,"about_ca_system_score_codex":0.001279873,"about_ca_system_score_gemma":0.0005172601,"threshold_uncertainty_score":0.02833885},"labels":[],"label_agreement":null},{"id":"W2027448964","doi":"10.1086/504584","title":"Radio Images of 3C 58: Expansion and Motion of Its Wisp","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Supernova remnant; Nebula; Physics; Astrophysics; Supernova; Pulsar; Limit (mathematics); Crab Nebula; Proper motion; Astronomy; Mathematics","score_opus":0.0065772521683331135,"score_gpt":0.2113804764507067,"score_spread":0.2048032242823736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027448964","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99528307,0.00009692314,0.00030097822,0.000037090234,0.000005794943,0.000008885388,0.00059932383,0.000057102312,0.003610819],"genre_scores_gemma":[0.9925062,0.00019741821,0.0023955489,0.00004590739,0.000023903658,0.000015892443,0.0028349939,0.00005639639,0.0019236607],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997306,9.2986545e-7,9.708442e-7,0.0000067264164,0.000009934498,0.000008475938],"domain_scores_gemma":[0.99987006,0.000010883568,0.000028747792,0.000014220037,0.000026197764,0.000049821363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000078741185,0.00015084949,0.00014897507,0.00097358326,0.00020525628,0.00020723023,0.00019629809,0.00022555135,0.0020938711],"category_scores_gemma":[0.00016268257,0.00011711048,0.000103463375,0.00041511114,0.00012523883,0.00011697666,0.00026078895,0.00034242676,0.0006221205],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093216216,0.00023292856,0.22680195,0.00011911063,0.00006207345,0.0038555868,0.00074523134,0.0012152308,0.69677347,0.0005289102,0.0055462,0.063187145],"study_design_scores_gemma":[0.00001671192,0.00007562268,0.99083215,0.0000122792035,0.000010696056,0.0010288804,0.0000785784,0.0010406398,0.0039906376,0.00004513936,0.0028623138,0.0000063481034],"about_ca_topic_score_codex":0.0044404846,"about_ca_topic_score_gemma":0.010855737,"teacher_disagreement_score":0.0044404846,"about_ca_system_score_codex":0.00020648292,"about_ca_system_score_gemma":0.00012724029,"threshold_uncertainty_score":0.008829296},"labels":[],"label_agreement":null},{"id":"W2027605453","doi":"10.1088/0004-637x/716/2/893","title":"MAGNETIC FIELD STRUCTURES AND TURBULENT COMPONENTS IN THE STAR-FORMING MOLECULAR CLOUDS OMC-2 AND OMC-3","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Polarization (electrochemistry); Physics; Astrophysics; Turbulence; Magnetic field; Position angle; Molecular cloud; Star formation; Protein filament; Galaxy; Stars; Meteorology; Materials science; Chemistry","score_opus":0.007873502176216296,"score_gpt":0.22652898423294543,"score_spread":0.21865548205672913,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027605453","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995993,0.000015386571,0.000023550785,0.00000811681,6.140528e-7,0.0000013748053,0.00013300224,0.0000044130884,0.00021419556],"genre_scores_gemma":[0.9992581,0.000012588827,0.00009509332,0.0000055110604,0.000002555615,0.0000026826149,0.0005616004,0.0000027906437,0.000059109854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999343,0.0000041546355,0.0000036028346,0.000012751056,0.000014892574,0.000030352845],"domain_scores_gemma":[0.99970204,0.0000309398,0.00010989423,0.000015449134,0.000049183378,0.00009240847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009192155,0.00017316462,0.00016269421,0.0008278093,0.00035929997,0.0004607502,0.00020378825,0.00020913698,0.00038145986],"category_scores_gemma":[0.00033248347,0.0001343252,0.00014072412,0.0008047316,0.0002411015,0.00013002165,0.0003342569,0.00022435604,0.00006301605],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042170574,0.000107060725,0.92437124,0.00002558288,0.000061739265,0.00037020922,0.00041789262,0.002979354,0.06525631,0.0005381607,0.0003951893,0.0050556306],"study_design_scores_gemma":[0.000005391066,0.000010211732,0.99794275,0.0000017248015,0.0000047611397,0.00002061784,0.00007635155,0.001333768,0.0004709249,0.00003164269,0.00009875265,0.000003061247],"about_ca_topic_score_codex":0.024091972,"about_ca_topic_score_gemma":0.02444564,"teacher_disagreement_score":0.024091972,"about_ca_system_score_codex":0.00076295267,"about_ca_system_score_gemma":0.00024615656,"threshold_uncertainty_score":0.04790348},"labels":[],"label_agreement":null},{"id":"W2027682369","doi":"10.1088/0004-637x/759/1/7","title":"HUNTING FOR THE PROGENITOR OF SN 1006: HIGH-RESOLUTION SPECTROSCOPIC SEARCH WITH THE FLAMES INSTRUMENT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Chandrasekhar limit; White dwarf; Supernova; Physics; Astrophysics; Accretion (finance); Astronomy; Thermonuclear fusion; Stars; Nuclear physics; Plasma","score_opus":0.014580455973141775,"score_gpt":0.24244386619991687,"score_spread":0.2278634102267751,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027682369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983891,0.000063548,0.00025192086,0.000018527719,0.0000031926756,0.00000987203,0.0003036929,0.000021858234,0.0009383357],"genre_scores_gemma":[0.9959741,0.0000849967,0.002051929,0.000016665295,0.0000066279476,0.0000039882516,0.0013056328,0.0000068570575,0.0005490775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993634,0.0000056433955,0.000004676674,0.000014749945,0.000025835856,0.000012689299],"domain_scores_gemma":[0.9996561,0.000035552643,0.00012087454,0.000028363127,0.000049899183,0.000109189066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003869363,0.00020867586,0.0002144667,0.0013863979,0.00045618258,0.00029925577,0.00028985614,0.00027130925,0.001069408],"category_scores_gemma":[0.0004748011,0.00013548358,0.00018750453,0.00065344275,0.00015477429,0.00024010544,0.00041685894,0.00016282426,0.00039002398],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041467143,0.00022676593,0.9259643,0.000040225175,0.000074353935,0.0014622908,0.00026534792,0.0004882349,0.049622387,0.00031505077,0.00087101455,0.020255376],"study_design_scores_gemma":[0.000022152779,0.00026269731,0.98000836,0.000013788491,0.000043550517,0.0036561938,0.0004257274,0.0035781271,0.008744591,0.000254899,0.0029733393,0.000016527263],"about_ca_topic_score_codex":0.0024850906,"about_ca_topic_score_gemma":0.0051143914,"teacher_disagreement_score":0.0024850906,"about_ca_system_score_codex":0.00015492001,"about_ca_system_score_gemma":0.00014108581,"threshold_uncertainty_score":0.0049412847},"labels":[],"label_agreement":null},{"id":"W2027698749","doi":"10.1088/0004-637x/705/1/226","title":"90 GHz AND 150 GHz OBSERVATIONS OF THE ORION M42 REGION. A SUBMILLIMETER TO RADIO ANALYSIS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Emissivity; Astrophysics; Green Bank Telescope; Telescope; James Clerk Maxwell Telescope; Wavelength; Spectral index; Molecular cloud; Stars; Astronomy; Optics; Star formation; Spectral line","score_opus":0.018752459924595583,"score_gpt":0.2362342448901927,"score_spread":0.2174817849655971,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027698749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9914944,0.0002507613,0.0011150886,0.0000643216,0.000015814738,0.000031285213,0.0013428299,0.00010366194,0.00558175],"genre_scores_gemma":[0.9852904,0.00014283948,0.0059890472,0.00016176728,0.000055080658,0.00007195405,0.0058922106,0.000053538555,0.0023431682],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997278,0.00002487413,0.000008260395,0.000100552585,0.000074144096,0.00006440209],"domain_scores_gemma":[0.9996742,0.000025521396,0.00006898695,0.00006806089,0.00006418312,0.000099008656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003994356,0.00030722303,0.00023299652,0.00088992144,0.0003673536,0.00043277626,0.00037906735,0.00032771332,0.0014879212],"category_scores_gemma":[0.00046282058,0.00028183273,0.0002723519,0.00062895,0.0001397922,0.00026548607,0.0006175908,0.00022956559,0.0003546907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005867738,0.00031155001,0.6208224,0.00014965962,0.00024257269,0.0008701343,0.0015992364,0.001530496,0.28926614,0.00084008666,0.002912098,0.08086879],"study_design_scores_gemma":[0.000016752792,0.000037636775,0.99330753,0.0000064649084,0.000018422905,0.00011557145,0.00005291832,0.0004625839,0.0016551351,0.000058348378,0.004263285,0.000005322541],"about_ca_topic_score_codex":0.0061895866,"about_ca_topic_score_gemma":0.012163207,"teacher_disagreement_score":0.0061895866,"about_ca_system_score_codex":0.0003321983,"about_ca_system_score_gemma":0.0002406229,"threshold_uncertainty_score":0.012307107},"labels":[],"label_agreement":null},{"id":"W2027712233","doi":"10.1088/0004-637x/773/2/90","title":"STELLAR VELOCITY DISPERSION MEASUREMENTS IN HIGH-LUMINOSITY QUASAR HOSTS AND IMPLICATIONS FOR THE AGN BLACK HOLE MASS SCALE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":221,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Supermassive black hole; Quasar; Velocity dispersion; Black hole (networking); Galaxy; Reverberation mapping; Intermediate-mass black hole; Binary black hole","score_opus":0.014737981617099848,"score_gpt":0.22406887977617132,"score_spread":0.20933089815907147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027712233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975005,0.0004900335,0.00047279208,0.00006678289,0.000013336875,0.000002905543,0.00018947995,0.000013704261,0.0012505719],"genre_scores_gemma":[0.9993862,0.000094252515,0.00011990653,0.000022061811,0.000019648023,0.000001382434,0.00010481988,0.0000040493082,0.00024764592],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998648,0.000023704155,0.000008935856,0.000042102954,0.000027432552,0.0000329511],"domain_scores_gemma":[0.9991941,0.00021611257,0.0002666525,0.00004718899,0.00010146637,0.00017445073],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005508037,0.00020874273,0.0002282336,0.0014079852,0.00037980633,0.0008929937,0.0003326049,0.0006186981,0.0025422291],"category_scores_gemma":[0.0012316986,0.00014922145,0.00012924167,0.0006270954,0.0004060862,0.00047577653,0.00052076986,0.00037167265,0.000570373],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024047845,0.000050268765,0.9514533,0.000018450355,0.000023294404,0.00011360524,0.00018479243,0.00009983456,0.041136842,0.0002999706,0.00012654884,0.0062525594],"study_design_scores_gemma":[0.0000053557455,0.00006656367,0.9967409,0.000005386736,0.000009965682,0.00018777394,0.00018871571,0.00017257368,0.0022504642,0.00022422624,0.00014534197,0.0000028524366],"about_ca_topic_score_codex":0.0006050008,"about_ca_topic_score_gemma":0.00092785654,"teacher_disagreement_score":0.0025422291,"about_ca_system_score_codex":0.00020569161,"about_ca_system_score_gemma":0.000062694235,"threshold_uncertainty_score":0.0085045695},"labels":[],"label_agreement":null},{"id":"W2027739765","doi":"10.1086/503769","title":"The Spatial Clustering of Ultraluminous Infrared Galaxies over 1.5 &lt; <i>z</i> &lt; 3","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; QSOS; Astronomy; Luminous infrared galaxy; Galaxy; Halo; Dark matter; Stellar mass; Redshift; Elliptical galaxy; Star formation","score_opus":0.00460975524471353,"score_gpt":0.19280708528861248,"score_spread":0.18819733004389896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027739765","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987218,0.00003955982,0.00011066285,0.000014910547,7.538911e-7,0.0000019866645,0.0003187666,0.000022804945,0.0007687959],"genre_scores_gemma":[0.99886274,0.000020711692,0.00015035585,0.00000981447,0.000002897093,0.0000025321651,0.0007096492,0.0000030115436,0.00023834135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988985,0.0000059350946,0.0000043706004,0.000023761468,0.000027813425,0.00004830048],"domain_scores_gemma":[0.9992093,0.00005143046,0.00043866027,0.000041890657,0.000100000034,0.0001585654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013739735,0.00015188118,0.00013950857,0.0012989541,0.00022441336,0.0004102953,0.0002474404,0.00021477343,0.0009874668],"category_scores_gemma":[0.00040343558,0.00009580413,0.00016969773,0.0010230182,0.0002122991,0.00019799457,0.00033656225,0.00018972845,0.00026670765],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009047452,0.000028488788,0.98262954,0.000013639952,0.00003643952,0.00008240321,0.00032195586,0.00034266338,0.009756764,0.00023999653,0.00041163075,0.0060459054],"study_design_scores_gemma":[7.818671e-7,0.000006466005,0.99939716,8.5750185e-7,0.0000033441509,0.000025770263,0.000025778301,0.00016489846,0.00024774476,0.00001319216,0.000112977046,0.000001097559],"about_ca_topic_score_codex":0.011319356,"about_ca_topic_score_gemma":0.016824275,"teacher_disagreement_score":0.011319356,"about_ca_system_score_codex":0.00046342958,"about_ca_system_score_gemma":0.00010998978,"threshold_uncertainty_score":0.022506952},"labels":[],"label_agreement":null},{"id":"W2027778512","doi":"10.1088/0004-637x/708/2/1335","title":"THE AGES, METALLICITIES, AND ALPHA ELEMENT ENHANCEMENTS OF GLOBULAR CLUSTERS IN THE ELLIPTICAL NGC 5128: A HOMOGENEOUS SPECTROSCOPIC STUDY WITH GEMINI/GEMINI MULTI-OBJECT SPECTROGRAPH","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Waterloo; McMaster University; University of British Columbia","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Metallicity; Galaxy; Elliptical galaxy; Milky Way; Stellar population; Population; Astronomy; Star formation; Medicine","score_opus":0.009450355099098166,"score_gpt":0.24283923449515024,"score_spread":0.23338887939605207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027778512","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997137,0.000015876585,0.000036077487,0.0000029816429,3.471196e-7,8.5908823e-7,0.000058713093,0.0000032529927,0.00016820934],"genre_scores_gemma":[0.9994037,0.000020761918,0.00015323228,0.000003712682,0.0000016472208,0.0000017634624,0.00018978753,0.0000018610676,0.00022348898],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991906,0.0000048672587,0.0000059893655,0.000036611087,0.000015686519,0.000017712748],"domain_scores_gemma":[0.99971837,0.000020995016,0.000096741715,0.00004452795,0.0000485715,0.00007064834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001332776,0.00021205391,0.0001263855,0.0006657372,0.00022122562,0.00021991039,0.00018918885,0.00013273161,0.00048153632],"category_scores_gemma":[0.0002476167,0.00013669598,0.00010387501,0.00041155907,0.0002285228,0.00026790827,0.00033803613,0.00010542625,0.00022242252],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011901223,0.000024509585,0.9654796,0.000007549321,0.000015301153,0.00017918304,0.00026321074,0.00014609563,0.030512309,0.000032353055,0.000059155387,0.0031617314],"study_design_scores_gemma":[0.0000020287673,0.000024981493,0.99859875,0.0000013504481,0.00000663544,0.00017033517,0.000080791506,0.00019901403,0.00075259944,0.000013717073,0.0001473944,0.0000024065982],"about_ca_topic_score_codex":0.004750551,"about_ca_topic_score_gemma":0.008758133,"teacher_disagreement_score":0.004750551,"about_ca_system_score_codex":0.00023645799,"about_ca_system_score_gemma":0.000058541053,"threshold_uncertainty_score":0.0094457865},"labels":[],"label_agreement":null},{"id":"W2027875010","doi":"10.1086/377119","title":"Locally Aromatic Polycyclic Hydrocarbons as Potential Carriers of Infrared Emission Features","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Diamond and Carbon-based Materials Research","field":"Materials Science","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Infrared; Infrared spectroscopy; Polycyclic aromatic hydrocarbon; Carbon fibers; Ionization; Aromaticity; Ion; Spectral line; Density functional theory; Analytical Chemistry (journal); Chemistry; Molecule; Computational chemistry; Materials science; Physics; Organic chemistry","score_opus":0.005753336446641569,"score_gpt":0.23929766862936164,"score_spread":0.23354433218272008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2027875010","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97257906,0.000473322,0.017383715,0.00013965709,0.000019821873,0.000029408619,0.00019126471,0.0001292768,0.009054542],"genre_scores_gemma":[0.992816,0.0001941175,0.006152998,0.000025086949,0.000005243227,0.000025749214,0.00013267061,0.000022134132,0.00062591594],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999285,0.000015222669,0.0000015658695,0.0000052019486,0.000032089487,0.000017426897],"domain_scores_gemma":[0.9998461,0.000074009455,0.000015687201,0.00001636465,0.000029040872,0.000018712664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016963106,0.0003336574,0.00027255138,0.0002560836,0.00029050934,0.00034591756,0.00052624656,0.0004266052,0.0018532658],"category_scores_gemma":[0.00031775076,0.00014280502,0.00022485801,0.00034495463,0.00035301532,0.00033563,0.00030210608,0.00045464994,0.00022423307],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040177192,0.00022024808,0.006903079,0.0007916411,0.000087095315,0.0010339713,0.0003148251,0.75888926,0.1466444,0.058310997,0.001463836,0.024938902],"study_design_scores_gemma":[0.000041892756,0.00009879084,0.0011945397,0.000011980975,0.000013980274,0.000061901075,0.000069203845,0.97514194,0.01791064,0.0048225736,0.0006172008,0.000015308593],"about_ca_topic_score_codex":0.0018235771,"about_ca_topic_score_gemma":0.0024692651,"teacher_disagreement_score":0.0018532658,"about_ca_system_score_codex":0.00036637645,"about_ca_system_score_gemma":0.00038795237,"threshold_uncertainty_score":0.006199777},"labels":[],"label_agreement":null},{"id":"W2028038703","doi":"10.1086/323438","title":"Astrometry with the MACHO Data Archive. I. High Proper Motion Stars toward the Galactic Bulge and Magellanic Clouds","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrometry; Proper motion; Stars; Photometry (optics); Bulge; Astrophysics; Astronomy; Milky Way; Galaxy; Light curve; Galactic Center","score_opus":0.018710382540215478,"score_gpt":0.22412717718517075,"score_spread":0.20541679464495527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028038703","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.05137756,0.0007968375,0.012055239,0.00067934603,0.00050434156,0.000793619,0.80736506,0.009044102,0.11738381],"genre_scores_gemma":[0.08067716,0.00049905665,0.028871996,0.00034877568,0.0003861167,0.0007366602,0.8700281,0.0012437386,0.017208492],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99846494,0.00011875304,0.00026122347,0.00026742072,0.00071470765,0.0001728468],"domain_scores_gemma":[0.9967012,0.00011415404,0.0007488415,0.0011144157,0.0010197656,0.00030149045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011116692,0.00079039455,0.00089440896,0.0056467606,0.00077972637,0.0015416889,0.0013443052,0.0005702334,0.031070067],"category_scores_gemma":[0.0038205178,0.0003697623,0.00054471375,0.0067860135,0.0002578672,0.0015168706,0.001982398,0.00094071176,0.035728868],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000779645,0.00028650754,0.12578486,0.0006804735,0.00020580273,0.00024313573,0.0005946674,0.0010736919,0.006658245,0.0051807356,0.6801817,0.17833054],"study_design_scores_gemma":[0.0001770816,0.00012940662,0.18794553,0.00010622399,0.00006958955,0.00024268903,0.00020450249,0.001876531,0.0024188645,0.0023176207,0.80446947,0.000042441177],"about_ca_topic_score_codex":0.008611109,"about_ca_topic_score_gemma":0.012772474,"teacher_disagreement_score":0.031070067,"about_ca_system_score_codex":0.00050305115,"about_ca_system_score_gemma":0.0011269512,"threshold_uncertainty_score":0.10393971},"labels":[],"label_agreement":null},{"id":"W2028071500","doi":"10.1086/591663","title":"The Origin of the Intrinsic Scatter in the Relation Between Black Hole Mass and Bulge Luminosity for Nearby Active Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Active galactic nucleus; Bulge; Galaxy; Black hole (networking); Quasar; Eddington luminosity; Virial theorem; Luminosity; Accretion (finance)","score_opus":0.013143959280143972,"score_gpt":0.22341331411789112,"score_spread":0.21026935483774714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028071500","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881303,0.00019118068,0.000559162,0.000016341834,0.000001668018,0.000001776109,0.0001749272,0.000013928036,0.00022803259],"genre_scores_gemma":[0.9994685,0.000032566564,0.00015369916,0.0000071620007,0.0000057482744,0.0000013419321,0.00028524685,0.0000033101012,0.00004248684],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99952817,0.0001374448,0.00004319538,0.00015643473,0.0000832994,0.00005145644],"domain_scores_gemma":[0.9933856,0.0026638708,0.0022414026,0.0010076495,0.00041571076,0.0002859102],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011706325,0.00023906198,0.00027816405,0.0017053767,0.00023586625,0.0007781038,0.00041358135,0.0003340368,0.00067538954],"category_scores_gemma":[0.0066717053,0.0001932257,0.00021322661,0.0008891913,0.0005353038,0.0004431739,0.00076769135,0.0001969383,0.00026760754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002433316,0.0000053585,0.9971033,0.00000478567,0.000035951518,0.000014165942,0.000103138125,0.0001386838,0.00088750344,0.000042184096,0.00002232238,0.0016182195],"study_design_scores_gemma":[0.0000010025376,0.000009685246,0.99900275,0.000001777004,0.000008338653,0.00006599767,0.000043876265,0.00048410532,0.0002513344,0.00006782209,0.000061295585,0.0000019918054],"about_ca_topic_score_codex":0.0021058444,"about_ca_topic_score_gemma":0.004187693,"teacher_disagreement_score":0.0021058444,"about_ca_system_score_codex":0.00023146563,"about_ca_system_score_gemma":0.00009038238,"threshold_uncertainty_score":0.0061909556},"labels":[],"label_agreement":null},{"id":"W2028261804","doi":"10.1088/0004-637x/767/1/45","title":"ASYMMETRY IN THE OUTBURST OF SN 1987A DETECTED USING LIGHT ECHO SPECTROSCOPY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Asymmetry; Physics; Spectroscopy; Ejecta; Supernova; Astrophysics; Position angle; Spectral line; Photosphere; Astronomy","score_opus":0.010525388621790092,"score_gpt":0.23720876469623367,"score_spread":0.22668337607444358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028261804","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99905366,0.00007092563,0.0003091954,0.000009067829,0.0000030749454,0.0000029945359,0.000093423114,0.000017859455,0.00043975606],"genre_scores_gemma":[0.99908185,0.000052785454,0.00035501955,0.000010083315,0.0000065484605,0.0000032297994,0.00029924168,0.000008645444,0.00018255506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990773,0.000008537826,0.0000047087624,0.000020076039,0.00003286307,0.00002592424],"domain_scores_gemma":[0.99945897,0.00007366216,0.00020491569,0.000034440636,0.00010299113,0.00012500577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021374015,0.00019394315,0.00015976469,0.0008259738,0.00018459544,0.00035189607,0.00017268563,0.00018201987,0.0005475403],"category_scores_gemma":[0.0005355135,0.00015554985,0.00015421979,0.00036908366,0.00018536426,0.00016138738,0.0003229392,0.00026342788,0.00017414187],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051879627,0.00007135017,0.68280166,0.000035236615,0.00007770089,0.00050608284,0.00037428393,0.00039088115,0.30600205,0.00023547791,0.00023124006,0.0087552555],"study_design_scores_gemma":[0.000004103328,0.00004913212,0.99245185,0.0000024740227,0.00001308632,0.00018567129,0.000047074394,0.0007027402,0.006240039,0.000054020184,0.00024537006,0.0000043269656],"about_ca_topic_score_codex":0.0020400234,"about_ca_topic_score_gemma":0.0039862837,"teacher_disagreement_score":0.0020400234,"about_ca_system_score_codex":0.00016666882,"about_ca_system_score_gemma":0.000121249024,"threshold_uncertainty_score":0.0040563345},"labels":[],"label_agreement":null},{"id":"W2028282243","doi":"10.1088/0004-637x/744/1/36","title":"COASTING EXTERNAL SHOCK IN WIND MEDIUM: AN ORIGIN FOR THE X-RAY PLATEAU DECAY COMPONENT IN<i>SWIFT</i>GAMMA-RAY BURST AFTERGLOWS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Ejecta; Physics; Astrophysics; Gamma-ray burst; Plateau (mathematics); Adiabatic process; Stars; Shock (circulatory); Lorentz factor; Light curve; Jet (fluid); Astronomy; Supernova; Mechanics; Lorentz transformation","score_opus":0.028636003105871482,"score_gpt":0.25474576160157714,"score_spread":0.22610975849570566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028282243","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985014,0.0001336587,0.0005116557,0.000016724644,0.0000022228585,0.000004348619,0.000051219886,0.000025135841,0.00075354445],"genre_scores_gemma":[0.999348,0.000055209865,0.00024031477,0.000010039669,0.0000036875806,0.0000029028408,0.00014373093,0.000008629187,0.00018735108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996734,0.0000018128488,0.0000025130948,0.000011098894,0.0000048445186,0.000012322741],"domain_scores_gemma":[0.9997782,0.000028743454,0.00009572739,0.000025427917,0.000026398116,0.000045535144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106530606,0.00020770004,0.00015388751,0.00038721357,0.00024108242,0.0006650666,0.00021929482,0.0002091005,0.0012749698],"category_scores_gemma":[0.0003008225,0.00014811178,0.00019507653,0.00027905207,0.00028270762,0.0002921904,0.00037512465,0.0002804697,0.00024057129],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047646876,0.00009552494,0.68972373,0.00009175671,0.00004579768,0.0017621554,0.00037314775,0.0008971391,0.29034925,0.0015537131,0.00024882331,0.014382589],"study_design_scores_gemma":[0.000022282184,0.00019766213,0.97604656,0.000017619954,0.000029762055,0.0013086353,0.00022163216,0.003576491,0.017251639,0.0005417954,0.0007732189,0.00001275242],"about_ca_topic_score_codex":0.00073544035,"about_ca_topic_score_gemma":0.00092636404,"teacher_disagreement_score":0.0012749698,"about_ca_system_score_codex":0.00016099283,"about_ca_system_score_gemma":0.000086553606,"threshold_uncertainty_score":0.004265189},"labels":[],"label_agreement":null},{"id":"W2028301746","doi":"10.1086/501041","title":"Correlation between Nuclear Spin Ratio of Cyclic C<sub>3</sub>H<sub>2</sub>and Chemical Evolution in TMC‐1 Cores","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Chemical Physics Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Spin (aerodynamics); Nuclear reaction; Nuclear physics; Astrophysics; Atomic physics; Thermodynamics","score_opus":0.0055021339528401065,"score_gpt":0.21466596780551173,"score_spread":0.20916383385267162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028301746","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994393,0.000034548717,0.00008721903,0.00000544712,9.775214e-7,0.0000020472298,0.00007614187,0.0000043009018,0.00035005022],"genre_scores_gemma":[0.99948263,0.000020408299,0.00015196107,0.0000065326335,0.0000021726914,0.000002736852,0.00018011765,0.000004929078,0.00014858709],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989104,0.0000072987896,0.000005480253,0.00004194023,0.000025993866,0.000028266037],"domain_scores_gemma":[0.9992142,0.000095869575,0.00028363446,0.00004400386,0.00023294831,0.00012928397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001770246,0.00017741056,0.00016291978,0.0008091678,0.00032987492,0.00034786228,0.0002650531,0.00021759525,0.0009817039],"category_scores_gemma":[0.00066756696,0.00024570752,0.0000866005,0.00038219386,0.0003923007,0.00024298785,0.00025162063,0.00023258457,0.0001756325],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004329918,0.000047593843,0.588217,0.000028106542,0.000058742982,0.00026486086,0.00027395642,0.0006637613,0.4055008,0.000265027,0.000104724786,0.0041424097],"study_design_scores_gemma":[0.000009788869,0.00008594335,0.9731724,0.0000016426267,0.00001377435,0.00014031076,0.00010955703,0.0014798847,0.0246857,0.00006900765,0.00022217238,0.000009905259],"about_ca_topic_score_codex":0.005862862,"about_ca_topic_score_gemma":0.0077732657,"teacher_disagreement_score":0.005862862,"about_ca_system_score_codex":0.00038052863,"about_ca_system_score_gemma":0.00014006173,"threshold_uncertainty_score":0.011657476},"labels":[],"label_agreement":null},{"id":"W2028383095","doi":"10.1088/0004-637x/704/2/1321","title":"<i>XMM-NEWTON</i>X-RAY DETECTION OF THE HIGH-MAGNETIC-FIELD RADIO PULSAR PSR B1916+14","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Physics; Neutron star; Astrophysics; Black-body radiation; Observatory; Magnetic field; X-ray pulsar; Astronomy; Radiation; Nuclear physics","score_opus":0.005372694885761966,"score_gpt":0.26245190068954855,"score_spread":0.25707920580378657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028383095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98920107,0.0012661848,0.0016528353,0.00026188837,0.00006999863,0.00003469674,0.0012175342,0.00013839705,0.0061574155],"genre_scores_gemma":[0.9898344,0.00057673623,0.00557857,0.00017879775,0.00013634606,0.000030073643,0.0021161488,0.00003499954,0.0015138912],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998914,0.000010567055,0.000016341886,0.00003758191,0.00003114444,0.000012980011],"domain_scores_gemma":[0.9990307,0.00008530903,0.0005503946,0.0001144215,0.00010489738,0.0001142039],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024346395,0.00038223507,0.00027671191,0.0009712656,0.00040946557,0.0004370562,0.00052334974,0.00036220535,0.0032895335],"category_scores_gemma":[0.0006807356,0.00015204637,0.00018738405,0.00059457374,0.00045916848,0.0003618749,0.00059896585,0.00029605022,0.00090800377],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068339077,0.00016316587,0.6285101,0.00043183638,0.00023669531,0.0019947602,0.00027715164,0.0002796963,0.31205156,0.00088617596,0.0024983264,0.051987067],"study_design_scores_gemma":[0.00006710207,0.0005453999,0.9132742,0.000060656814,0.00012313895,0.008955999,0.000078946425,0.0005996779,0.058374215,0.0007636609,0.017125642,0.000031414853],"about_ca_topic_score_codex":0.00053833955,"about_ca_topic_score_gemma":0.0015612273,"teacher_disagreement_score":0.0032895335,"about_ca_system_score_codex":0.00022429571,"about_ca_system_score_gemma":0.000121663055,"threshold_uncertainty_score":0.011004567},"labels":[],"label_agreement":null},{"id":"W2028441133","doi":"10.1086/339511","title":"Gravitational Bending of Light Near Compact Objects","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":302,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Schwarzschild radius; Antipodal point; Pulsar; Black-body radiation; Neutron star; RADIUS; Compact star; Schwarzschild metric; Amplitude","score_opus":0.018398396741763946,"score_gpt":0.30635521985504427,"score_spread":0.2879568231132803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028441133","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9362759,0.00137091,0.03653506,0.00022887066,0.000059902788,0.000021641417,0.00007652052,0.00037625694,0.025054999],"genre_scores_gemma":[0.9958759,0.00034253558,0.0014924303,0.000044421406,0.000038770657,0.000007659254,0.00005538476,0.000045229164,0.0020976726],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99990654,0.000018286253,0.000003485296,0.000019405192,0.00003250973,0.000019765894],"domain_scores_gemma":[0.9997743,0.000058044985,0.00006437321,0.000033341013,0.000024533578,0.00004545968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015033198,0.00052691484,0.00024474494,0.00057910394,0.00030312623,0.00058213907,0.0003854502,0.00042472707,0.0019493928],"category_scores_gemma":[0.0006999559,0.00021235945,0.00030275827,0.00037355194,0.0006506432,0.00040118778,0.0008511604,0.00046957727,0.0004680413],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007872417,0.00009191257,0.017794047,0.0003770644,0.0001527084,0.0039403327,0.0014490448,0.1436801,0.6476561,0.121894024,0.0018477303,0.0603297],"study_design_scores_gemma":[0.00014440763,0.0011642115,0.14245792,0.00014722635,0.00017612989,0.007693053,0.00092208496,0.59584075,0.08422938,0.15581141,0.01107139,0.0003420406],"about_ca_topic_score_codex":0.0007608638,"about_ca_topic_score_gemma":0.0003903401,"teacher_disagreement_score":0.0019493928,"about_ca_system_score_codex":0.00051060726,"about_ca_system_score_gemma":0.00009944314,"threshold_uncertainty_score":0.006521404},"labels":[],"label_agreement":null},{"id":"W2028548470","doi":"10.1088/0004-637x/712/1/250","title":"A STUDY OF VEGA: A RAPIDLY ROTATING POLE-ON STAR","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Microturbulence; Astrophysics; Photosphere; Polar; Spectral line; Stars; Spectroscopy; Effective temperature; Astronomy","score_opus":0.012115990675002186,"score_gpt":0.2432980914227881,"score_spread":0.23118210074778592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028548470","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998566,0.0000646365,0.000106304266,0.000013209048,0.0000040763457,0.0000059165404,0.0000736087,0.00000567703,0.0011606838],"genre_scores_gemma":[0.99873775,0.000043461343,0.00023419659,0.000024190964,0.0000054376105,0.0000030567603,0.00031338845,0.0000043139803,0.0006342532],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999219,0.000012189523,0.00000294784,0.00002460633,0.00001396081,0.000024387755],"domain_scores_gemma":[0.9998356,0.000026057553,0.000024698926,0.000023435085,0.000022074175,0.00006816361],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011572132,0.00029288797,0.00028507484,0.0006104221,0.0009165835,0.0004391935,0.0003037963,0.0004104381,0.0005337478],"category_scores_gemma":[0.00022837707,0.00013735739,0.00023286993,0.0003988907,0.0004091938,0.00021121367,0.00035907587,0.00029434584,0.00035183132],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014175369,0.0008908182,0.54805964,0.00017334126,0.00022324784,0.006623854,0.0027586103,0.0030766495,0.40117276,0.002929235,0.0017403838,0.030933976],"study_design_scores_gemma":[0.000023260596,0.0011157284,0.98262995,0.000011623374,0.000022153272,0.0036476601,0.0008177621,0.001656135,0.004814726,0.00025449635,0.0049928427,0.000013749848],"about_ca_topic_score_codex":0.005255413,"about_ca_topic_score_gemma":0.0073597413,"teacher_disagreement_score":0.005255413,"about_ca_system_score_codex":0.00033764192,"about_ca_system_score_gemma":0.00013566391,"threshold_uncertainty_score":0.010449648},"labels":[],"label_agreement":null},{"id":"W2028571339","doi":"10.1086/512229","title":"Variability of 19 Millisecond Pulsars in 47 Tucanae with<i>Chandra</i>HRC‐S","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Globular cluster; Millisecond pulsar; Neutron star; Observatory; Pulsar; Millisecond; Astronomy; Magnetosphere; Cluster (spacecraft); Binary number; Duty cycle; Magnetic field; Stars","score_opus":0.008173936264505056,"score_gpt":0.29670041335628483,"score_spread":0.28852647709177975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028571339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984413,0.000092231654,0.00006741277,0.000025684623,0.0000031009401,0.0000045214338,0.00051401125,0.00002200911,0.0008297498],"genre_scores_gemma":[0.9978994,0.000077020835,0.00024157189,0.000019479841,0.000008975279,0.00000913736,0.0015110071,0.000016576532,0.00021691507],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973565,0.000012086969,0.000007123087,0.00006359513,0.000060764836,0.00012068061],"domain_scores_gemma":[0.99946946,0.000055663124,0.00015693252,0.000057650766,0.00014209442,0.00011824229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027058646,0.0002925213,0.00047849264,0.0013795247,0.0012562122,0.0013026033,0.0007790768,0.00038337838,0.0008715994],"category_scores_gemma":[0.0005947582,0.00015699344,0.00033929903,0.0020959927,0.00043147313,0.00025798968,0.00069633883,0.0003967656,0.00016361674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051993295,0.00016951942,0.9351813,0.00004856234,0.00037388736,0.00056152034,0.0009418101,0.005167507,0.02773773,0.0007513567,0.0028264315,0.025720421],"study_design_scores_gemma":[0.000015580223,0.0000272054,0.9921976,0.000009885851,0.000059091744,0.00011323969,0.00027564846,0.0027800112,0.0016918038,0.00006066066,0.0027490505,0.000020227113],"about_ca_topic_score_codex":0.2019544,"about_ca_topic_score_gemma":0.21443237,"teacher_disagreement_score":0.2019544,"about_ca_system_score_codex":0.0018651498,"about_ca_system_score_gemma":0.0011260809,"threshold_uncertainty_score":0.4015578},"labels":[],"label_agreement":null},{"id":"W2028731813","doi":"10.1088/0004-637x/767/1/61","title":"IN SEARCH OF DUST CLOUDS: PHOTOMETRIC MONITORING OF A SAMPLE OF LATE L AND T DWARFS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"Shanghai Municipal Education Commission; National Natural Science Foundation of China","keywords":"Physics; Brown dwarf; Astrophysics; Photosphere; Light curve; Photometry (optics); Amplitude; Flux (metallurgy); Astronomy; Periodogram; Rotation period; Stars; Spectral line","score_opus":0.019439704630606378,"score_gpt":0.2560872771517753,"score_spread":0.23664757252116894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028731813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999683,0.000021454356,0.000092394286,0.000004819629,5.148213e-7,0.0000021883254,0.00007511029,0.000005140489,0.00011540798],"genre_scores_gemma":[0.99940383,0.000013909387,0.00020177788,0.0000062712043,0.000002567316,0.0000022903141,0.00025443727,0.0000015190028,0.00011347646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984896,0.000021778336,0.000010804464,0.000055335608,0.000027191707,0.000035827834],"domain_scores_gemma":[0.99954444,0.000041994244,0.00011569047,0.000037567865,0.000076288496,0.00018403938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023871119,0.0001455776,0.00019304173,0.0009256989,0.0003123647,0.0003207227,0.00016997334,0.00017182136,0.00024921304],"category_scores_gemma":[0.0004388462,0.00007475136,0.00012757037,0.00054082857,0.00017499311,0.00015977368,0.00032650863,0.0001083744,0.00015456456],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001341848,0.000047369886,0.9749714,0.000009375862,0.000014460288,0.00012973626,0.000372251,0.000083823004,0.019776141,0.000036809048,0.00009354467,0.0043308693],"study_design_scores_gemma":[0.000002047961,0.000042533702,0.99877375,5.191377e-7,0.0000035092344,0.0001008624,0.00011048248,0.00017972953,0.0006660872,0.0000095947335,0.00010994265,9.668008e-7],"about_ca_topic_score_codex":0.0040345006,"about_ca_topic_score_gemma":0.007819291,"teacher_disagreement_score":0.0040345006,"about_ca_system_score_codex":0.00017656306,"about_ca_system_score_gemma":0.00015064553,"threshold_uncertainty_score":0.00802201},"labels":[],"label_agreement":null},{"id":"W2028870418","doi":"10.1086/378798","title":"Theoretical Considerations on the Properties of Accreting Millisecond Pulsars","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Millisecond pulsar; Physics; Astrophysics; Accretion (finance); Angular momentum; Orbital period; Binary number; Millisecond; Pulsar; Orbital inclination; Stars; Astronomy; Classical mechanics","score_opus":0.022443946772291386,"score_gpt":0.22493952170719855,"score_spread":0.20249557493490716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028870418","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90397346,0.000963489,0.052913524,0.00185467,0.00005005224,0.0000384637,0.0004882287,0.00026046563,0.039457582],"genre_scores_gemma":[0.99530435,0.00041264438,0.0024955408,0.00008335546,0.000038616814,0.000037014735,0.00019774289,0.000036950754,0.0013938622],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99985814,0.000029194754,0.000006172845,0.000022238724,0.000044494103,0.000039788483],"domain_scores_gemma":[0.99844116,0.001069734,0.00021313808,0.00009851069,0.00009620923,0.00008124943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007795488,0.00045436248,0.00045485565,0.00087676203,0.0012034859,0.0014506052,0.0014445626,0.00096795056,0.0045027165],"category_scores_gemma":[0.0060520032,0.00035893967,0.0007490262,0.00077848096,0.00088854163,0.0021596989,0.00079321116,0.0007186592,0.000467482],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000073400166,0.000062628074,0.033402964,0.000111874506,0.00004658622,0.00062453357,0.0003000574,0.77472675,0.0024205036,0.18038204,0.00081235997,0.007036312],"study_design_scores_gemma":[0.000037469315,0.00006337759,0.013936424,0.000036396912,0.00003149809,0.00034314772,0.00020693359,0.8684769,0.0009074617,0.11462143,0.0013117498,0.000027282238],"about_ca_topic_score_codex":0.003433901,"about_ca_topic_score_gemma":0.0017138369,"teacher_disagreement_score":0.0045027165,"about_ca_system_score_codex":0.0011048838,"about_ca_system_score_gemma":0.00050941086,"threshold_uncertainty_score":0.015063107},"labels":[],"label_agreement":null},{"id":"W2028874878","doi":"10.1088/0004-637x/690/2/1045","title":"D/H ALONG THE LINE OF SIGHT OF REJ 1738+665","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency","funders":"","keywords":"Physics; Stars; Line-of-sight; Astrophysics; Spectral line; Line (geometry); Absorption spectroscopy; Local Bubble; Interstellar medium; Astronomy; Geometry; Optics; Galaxy","score_opus":0.015316241147645395,"score_gpt":0.22341050107400703,"score_spread":0.20809425992636163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028874878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8722429,0.00097401947,0.001179886,0.0018150075,0.00067067984,0.00008805354,0.016665298,0.00074207195,0.10562215],"genre_scores_gemma":[0.9797773,0.00027728584,0.0009591675,0.00044420752,0.00019173081,0.000020446214,0.006667264,0.00012306316,0.011539444],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989295,0.0000065911972,0.0000026256178,0.000029920298,0.000023650357,0.000044351527],"domain_scores_gemma":[0.9997949,0.000014187246,0.00003958277,0.000011794799,0.000052726195,0.000086859196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016645378,0.00045163362,0.0004164854,0.00084883586,0.0006031799,0.0004840862,0.0003629025,0.00068287435,0.011160451],"category_scores_gemma":[0.00021887703,0.00012405573,0.00026731534,0.00078307075,0.0001592037,0.00028498244,0.0003459835,0.0005540692,0.002143592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0033088054,0.00045452037,0.486724,0.00063705916,0.00031357433,0.0049596266,0.0009220194,0.007315614,0.25759542,0.0052459287,0.1354173,0.097106144],"study_design_scores_gemma":[0.000052032774,0.00008629538,0.9694914,0.000021770793,0.0000394996,0.00023947061,0.0003266069,0.001484431,0.002461429,0.0003488653,0.025425425,0.000022638667],"about_ca_topic_score_codex":0.016256202,"about_ca_topic_score_gemma":0.021048207,"teacher_disagreement_score":0.016256202,"about_ca_system_score_codex":0.0005410028,"about_ca_system_score_gemma":0.0003128493,"threshold_uncertainty_score":0.037335455},"labels":[],"label_agreement":null},{"id":"W2028901308","doi":"10.1086/368109","title":"The Canada‐UK Deep Submillimeter Survey. VI. The 3 Hour Field","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"James Clerk Maxwell Telescope; Physics; Astrophysics; Redshift; Galaxy; Astronomy; Telescope; Submillimeter Array; Flux (metallurgy); Bolometer; Hubble Deep Field; Cosmic microwave background; Star formation; Optics","score_opus":0.0070636460062439965,"score_gpt":0.19543240515234445,"score_spread":0.18836875914610046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028901308","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14602181,0.0028735765,0.0014140672,0.0016775656,0.0002587441,0.0002891708,0.7686139,0.00056684966,0.07828444],"genre_scores_gemma":[0.4500977,0.0033366203,0.0061705615,0.0017953104,0.00012041091,0.00038395988,0.40489548,0.00037372616,0.13282628],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.999592,0.000014886055,0.0000134092425,0.00004344205,0.00015992057,0.00017632295],"domain_scores_gemma":[0.9982267,0.000056581946,0.00025015316,0.00013700021,0.0008521242,0.0004774207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024337485,0.00032631846,0.0002615701,0.0021698189,0.0007814826,0.0007747093,0.00058771914,0.00030007487,0.015882688],"category_scores_gemma":[0.00073403964,0.00019168445,0.00022823775,0.0041197543,0.0002351654,0.00035161167,0.0005931728,0.00047949076,0.0046376903],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030763543,0.000055592034,0.27473253,0.0002900862,0.00007315105,0.00018352906,0.0007930845,0.00040884613,0.0024901333,0.0033436706,0.64134264,0.07597906],"study_design_scores_gemma":[0.000015495927,0.000012386352,0.7693919,0.00005472991,0.000009574316,0.0000527283,0.00029702566,0.00020289922,0.0002766996,0.0001326291,0.22953703,0.00001701252],"about_ca_topic_score_codex":0.9553902,"about_ca_topic_score_gemma":0.9795751,"teacher_disagreement_score":0.044609785,"about_ca_system_score_codex":0.0061775222,"about_ca_system_score_gemma":0.009121947,"threshold_uncertainty_score":0.089744925},"labels":[],"label_agreement":null},{"id":"W2028945692","doi":"10.1086/308683","title":"Structure and Stability of Keplerian Magnetohydrodynamic Jets","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Magnetohydrodynamics; Magnetohydrodynamic drive; Jet (fluid); Rotational symmetry; Angular momentum; Mechanics; Rotation (mathematics); Linear stability; Current (fluid); Nonlinear system; Classical mechanics; Core (optical fiber); Vortex; Work (physics); Instability; Magnetic field; Geometry; Optics","score_opus":0.00557750467940521,"score_gpt":0.21175424493611478,"score_spread":0.20617674025670957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028945692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99538404,0.00008778888,0.002024406,0.00006732278,0.0000036689135,0.0000051249963,0.000041917592,0.000036671314,0.0023491262],"genre_scores_gemma":[0.9995024,0.000021789276,0.000211325,0.0000040075442,0.0000022621387,0.000002626483,0.000022405366,0.0000055126393,0.00022759924],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999293,0.000014949191,0.0000045243955,0.000015946995,0.00001531877,0.000019892062],"domain_scores_gemma":[0.99961543,0.0001339268,0.000105969586,0.000027507016,0.00005904973,0.000058078946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017387955,0.0002203524,0.00028486783,0.0004837418,0.00053165836,0.0010965378,0.00039241492,0.0004603695,0.000806796],"category_scores_gemma":[0.0016076259,0.00023414163,0.0002221131,0.00022774107,0.0008149123,0.00062419806,0.0004746954,0.00030813116,0.0001466771],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004415844,0.00015444319,0.03683272,0.000056628327,0.00006476731,0.00046595724,0.00065196,0.8881183,0.040229157,0.02665713,0.00064235134,0.0056849807],"study_design_scores_gemma":[0.0000342381,0.000038876293,0.008606616,0.000004864097,0.000006750142,0.0000495439,0.00006031502,0.9854525,0.0016836254,0.0038665743,0.0001790885,0.000017022341],"about_ca_topic_score_codex":0.0037443978,"about_ca_topic_score_gemma":0.001049538,"teacher_disagreement_score":0.0037443978,"about_ca_system_score_codex":0.00089083984,"about_ca_system_score_gemma":0.00035845066,"threshold_uncertainty_score":0.007445216},"labels":[],"label_agreement":null},{"id":"W2028967072","doi":"10.1086/367852","title":"Infrared Absorption Spectra of Deuterated Amorphous Carbon","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Quantum, superfluid, helium dynamics","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Deuterium; Spectral line; Infrared spectroscopy; Absorption (acoustics); Astrophysics; Absorption spectroscopy; Carbon star; Infrared; Amorphous carbon; Amorphous solid; Astronomy; Carbon fibers; Astrobiology; Atomic physics; Optics; Raman spectroscopy; Materials science; Crystallography","score_opus":0.00653565625979158,"score_gpt":0.21186687551440023,"score_spread":0.20533121925460865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2028967072","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99291515,0.00092224864,0.0021429115,0.0000319945,0.000031932075,0.0000130956005,0.00042112873,0.00005325985,0.0034682786],"genre_scores_gemma":[0.99565434,0.00045173566,0.001683574,0.00003354763,0.000011296887,0.000009040578,0.00050894864,0.000017042732,0.001630603],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998903,0.000010169984,0.000006252049,0.000026238926,0.000042595224,0.000024505767],"domain_scores_gemma":[0.9997944,0.00004758572,0.00003169321,0.000028235367,0.000074107964,0.000023895951],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012298649,0.00020670195,0.00014490756,0.00041833104,0.0003550317,0.00018523671,0.00021640472,0.0002344175,0.0019149265],"category_scores_gemma":[0.00018889036,0.00008572333,0.0001036764,0.00032123466,0.00022895528,0.00015945698,0.000096351454,0.00032389566,0.00019084247],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055892135,0.000009485126,0.00027888615,0.000024857063,0.000005329571,0.00004050313,0.000015669395,0.000077194505,0.99869126,0.00004965814,0.000036483267,0.0007147411],"study_design_scores_gemma":[0.000006472809,0.00009160972,0.005746595,0.000004494582,0.000010698618,0.00009761173,0.000025992647,0.00041718906,0.99219006,0.00003611693,0.0013659563,0.0000071328677],"about_ca_topic_score_codex":0.0007457361,"about_ca_topic_score_gemma":0.0006459767,"teacher_disagreement_score":0.0019149265,"about_ca_system_score_codex":0.00014657727,"about_ca_system_score_gemma":0.00006781234,"threshold_uncertainty_score":0.006406069},"labels":[],"label_agreement":null},{"id":"W2029120438","doi":"10.1086/368258","title":"On the Total Energy of Open Friedmann‐Robertson‐Walker Universes","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Northern British Columbia","funders":"","keywords":"Friedmann–Lemaître–Robertson–Walker metric; Minkowski space; Universe; De Sitter space; De Sitter universe; Einstein field equations; Total energy; Zero (linguistics); Gravitational field; Cosmology","score_opus":0.00885584360001197,"score_gpt":0.23688118954988094,"score_spread":0.22802534594986898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029120438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.80171937,0.0064171613,0.04396799,0.0021245228,0.00027946426,0.000024791327,0.0003277803,0.000073354524,0.14506549],"genre_scores_gemma":[0.98412365,0.0016628765,0.0024695236,0.000103856764,0.00026584437,0.0000332538,0.00016939935,0.000053164207,0.011118506],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997421,0.000076247794,0.000013502733,0.000028741757,0.00008761925,0.00005180393],"domain_scores_gemma":[0.9994778,0.00022357334,0.00007181632,0.00004929743,0.00008877541,0.00008870162],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007022052,0.00052788685,0.00054680416,0.0017289426,0.0012540675,0.0018944317,0.0007509506,0.00055542385,0.0037066506],"category_scores_gemma":[0.0018119446,0.00031769622,0.00041862228,0.0007681026,0.0030825313,0.0026492116,0.001644819,0.0007724366,0.00033817912],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027486367,0.000010158509,0.00037124474,0.00002940334,0.000014017471,0.00006208661,0.00011903924,0.004002246,0.00077157334,0.9914624,0.00047519867,0.0026551385],"study_design_scores_gemma":[0.000011791519,0.000014588159,0.0013533015,0.000022644455,0.000007971575,0.00007768951,0.00008796577,0.012410393,0.00022286105,0.9841785,0.0015983889,0.0000140521115],"about_ca_topic_score_codex":0.0013395854,"about_ca_topic_score_gemma":0.0012520654,"teacher_disagreement_score":0.0037066506,"about_ca_system_score_codex":0.0009372297,"about_ca_system_score_gemma":0.00038335024,"threshold_uncertainty_score":0.012400031},"labels":[],"label_agreement":null},{"id":"W2029142394","doi":"10.1086/367823","title":"Interactions between a Bright Young Stellar Object and the<i>Midcourse Space Experiment</i>Infrared‐dark Cloud G79.3+0.3: An Early Stage of Triggered Star Formation?","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Young stellar object; Millimeter; Star formation; Molecular cloud; Infrared; Star (game theory); Protostar; Space observatory","score_opus":0.01197894861529717,"score_gpt":0.26010108125262404,"score_spread":0.24812213263732688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029142394","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992361,0.000050330822,0.000039717528,0.000056831672,0.0000022003735,0.0000023205714,0.000011083884,0.000003489296,0.0005981013],"genre_scores_gemma":[0.99952626,0.000032499753,0.0000718849,0.00004098285,0.000010053955,0.0000014434977,0.000030865107,8.772774e-7,0.0002852089],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999454,0.000007377068,0.0000020511964,0.000008035778,0.000007330103,0.000029896226],"domain_scores_gemma":[0.999691,0.000053924337,0.000110550835,0.000017835535,0.000018796392,0.00010784924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001462733,0.00008757011,0.00017367325,0.00022788005,0.00050027843,0.0005137907,0.00015324571,0.00054983806,0.0017410517],"category_scores_gemma":[0.00047311187,0.00010926795,0.000109854045,0.00014075634,0.00021247893,0.00033034763,0.0002981369,0.00021381435,0.0003529371],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039368702,0.00017111498,0.95052385,0.000016435351,0.000028766204,0.0022471545,0.00036123788,0.0000877208,0.03625583,0.0005142558,0.00036532842,0.009034618],"study_design_scores_gemma":[0.000011628224,0.0001292556,0.99587965,0.0000038068308,0.000014913047,0.0012272486,0.0003780246,0.00023566294,0.001372135,0.00025064667,0.000491812,0.00000525721],"about_ca_topic_score_codex":0.0025344386,"about_ca_topic_score_gemma":0.0058087083,"teacher_disagreement_score":0.0025344386,"about_ca_system_score_codex":0.00027613103,"about_ca_system_score_gemma":0.00013599536,"threshold_uncertainty_score":0.005824387},"labels":[],"label_agreement":null},{"id":"W2029190898","doi":"10.1088/0004-637x/745/1/18","title":"HOW STARLESS ARE STARLESS CORES?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Astrophysics; Physics; Millimeter; Infrared; Outflow; Core (optical fiber); Luminosity; Astronomy; High resolution; Star formation; Stars; Remote sensing; Optics","score_opus":0.027436558275635202,"score_gpt":0.226676684632816,"score_spread":0.1992401263571808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029190898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9859504,0.0045467084,0.0018320632,0.001524457,0.00008534348,0.000014892026,0.00019144795,0.000020585987,0.0058342326],"genre_scores_gemma":[0.99830186,0.00056309317,0.00023876883,0.00027161924,0.000037561946,0.000001831207,0.000061442726,0.0000057885777,0.0005179086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962425,0.00009628696,0.000032331573,0.00010964346,0.0000786387,0.000058812857],"domain_scores_gemma":[0.9959364,0.0008833963,0.0016484786,0.00027787374,0.00053545315,0.00071833347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008771055,0.00016697805,0.00039180435,0.00081749767,0.0003846016,0.0015657546,0.00040909008,0.00049577834,0.002223609],"category_scores_gemma":[0.0098897405,0.00012379693,0.0001278529,0.00050868234,0.0018072985,0.0024363524,0.00059321546,0.00030372996,0.0006857632],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006932099,0.00011253598,0.81799567,0.00033017053,0.00015514717,0.0015927346,0.0036928663,0.0006385631,0.00730955,0.014734835,0.0025133025,0.15023136],"study_design_scores_gemma":[0.00009376128,0.00055996195,0.83537334,0.00034931605,0.00015308554,0.010838602,0.0113761015,0.0020994851,0.0046835034,0.106347255,0.02805825,0.00006734945],"about_ca_topic_score_codex":0.0012741188,"about_ca_topic_score_gemma":0.0017951252,"teacher_disagreement_score":0.002223609,"about_ca_system_score_codex":0.0003322712,"about_ca_system_score_gemma":0.00028203783,"threshold_uncertainty_score":0.0074387193},"labels":[],"label_agreement":null},{"id":"W2029195105","doi":"10.1088/0004-637x/729/1/2","title":"SPECTRAL ENERGY DISTRIBUTION OF MARKARIAN 501: QUIESCENT STATE VERSUS EXTREME OUTBURST","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation; Science Foundation Ireland; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; U.S. Department of Energy; Smithsonian Institution","keywords":"Physics; Astrophysics; Blazar; Spectral energy distribution; Fermi Gamma-ray Space Telescope; Luminosity; Active galactic nucleus; Gamma ray; Astronomy; Flux (metallurgy); Synchrotron; Galaxy","score_opus":0.021954763842750587,"score_gpt":0.20794921162652774,"score_spread":0.18599444778377716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029195105","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988501,0.000027088228,0.0001073121,0.000009898983,7.9854203e-7,0.0000013672868,0.00012300613,0.000011014485,0.0008693168],"genre_scores_gemma":[0.99942565,0.0000139852955,0.00006893882,0.0000069647917,0.0000023922235,0.0000010875675,0.00030823864,0.000005029039,0.00016775819],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992275,0.000005839384,0.0000055802534,0.000028779072,0.000014889107,0.0000221077],"domain_scores_gemma":[0.99952924,0.000088041386,0.00018443755,0.000040296443,0.00004876084,0.000109286884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013288447,0.000110572786,0.0001837716,0.00084968517,0.00022565223,0.0005784117,0.00025139403,0.00022552081,0.0011255421],"category_scores_gemma":[0.00047799211,0.00011293934,0.00011502909,0.00045035873,0.0003137534,0.00026905967,0.0003850831,0.00016464574,0.0002529202],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057001045,0.000067761364,0.9143142,0.00002496446,0.000050907878,0.00044698798,0.00068552134,0.0005356862,0.07239933,0.0007197894,0.00041208536,0.009772765],"study_design_scores_gemma":[0.0000022132494,0.000019849842,0.997846,0.0000015925955,0.000006044473,0.00011660382,0.0000882782,0.00039431124,0.0013296588,0.000059392623,0.00013222966,0.0000038481626],"about_ca_topic_score_codex":0.0020763979,"about_ca_topic_score_gemma":0.003440879,"teacher_disagreement_score":0.0020763979,"about_ca_system_score_codex":0.00032788957,"about_ca_system_score_gemma":0.00006315839,"threshold_uncertainty_score":0.0041285753},"labels":[],"label_agreement":null},{"id":"W2029304706","doi":"10.1088/0004-637x/700/2/1794","title":"THE VELOCITY DISTRIBUTION OF NEARBY STARS FROM<i>HIPPARCOS</i>DATA. I. THE SIGNIFICANCE OF THE MOVING GROUPS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of New Brunswick","funders":"","keywords":"Stars; Radial velocity; Physics; Astrophysics; Gaussian; Distribution (mathematics); Mathematics; Mathematical analysis","score_opus":0.01251329860921396,"score_gpt":0.22455698817538522,"score_spread":0.21204368956617126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029304706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931988,0.00017692296,0.0035563707,0.000036848473,0.000004218082,0.0000043408813,0.0014700673,0.00018426977,0.0013679918],"genre_scores_gemma":[0.99213034,0.000059194565,0.0022792057,0.000007098523,0.000006619852,0.0000024158373,0.005291459,0.00003571154,0.00018788471],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998609,0.000019423782,0.000010734589,0.000056001638,0.00003817585,0.000014762495],"domain_scores_gemma":[0.9994492,0.00009526973,0.00020870233,0.00010780659,0.00007637811,0.000062589024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033267087,0.00014062633,0.00012661866,0.0012421487,0.00017615712,0.0004798156,0.00020257241,0.00025369978,0.0007627492],"category_scores_gemma":[0.0016616241,0.00009039031,0.00021051039,0.00089147367,0.00025655815,0.0003614646,0.00040497282,0.0002555331,0.0004642407],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020096907,0.00002616364,0.90889764,0.00007011463,0.00012007633,0.00008601084,0.0006617524,0.022649042,0.01487923,0.0022499657,0.0018179379,0.048340954],"study_design_scores_gemma":[0.000007937693,0.000022061158,0.9760893,0.0000099041745,0.000018586485,0.00012112504,0.00008528203,0.01895978,0.002005562,0.00065721595,0.0020064362,0.000016792468],"about_ca_topic_score_codex":0.00785641,"about_ca_topic_score_gemma":0.007884201,"teacher_disagreement_score":0.00785641,"about_ca_system_score_codex":0.0004215299,"about_ca_system_score_gemma":0.00018772582,"threshold_uncertainty_score":0.015621364},"labels":[],"label_agreement":null},{"id":"W2029420249","doi":"10.1086/428087","title":"Discovery of Two Gravitationally Lensed Quasars with Image Separations of 3″ from the Sloan Digital Sky Survey","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; York University; University of Toronto","funders":"","keywords":"Quasar; Physics; Astrophysics; Galaxy; Sky; Redshift; Lens (geology); Gravitational lens; Cosmology; Astronomy; Optics","score_opus":0.008937154606077548,"score_gpt":0.23298915461027217,"score_spread":0.22405200000419462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029420249","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99860615,0.00018004896,0.00028760772,0.000053155873,0.0000073499386,0.000006937029,0.0003279581,0.000030615865,0.0005002195],"genre_scores_gemma":[0.9968532,0.000106496445,0.0013220301,0.000059490812,0.000014711198,0.0000069893745,0.0012972902,0.0000057853067,0.00033399742],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955434,0.000021553307,0.000027212434,0.00010335174,0.00015846988,0.00013505458],"domain_scores_gemma":[0.99860626,0.00013625345,0.00056421384,0.00013059203,0.00016178304,0.0004008318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050516805,0.0003648691,0.00035338823,0.0019048786,0.0007133312,0.001032003,0.0003915241,0.00049128145,0.00066658924],"category_scores_gemma":[0.0008115055,0.00034580744,0.00028265265,0.0013622092,0.00046725117,0.00040143033,0.0012040737,0.000459795,0.00021221938],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027976953,0.00014339876,0.90813684,0.00007974131,0.00017051726,0.003955325,0.0011348061,0.00020931041,0.06306839,0.0007758876,0.0012064434,0.02083963],"study_design_scores_gemma":[0.000021396067,0.0000861626,0.9886397,0.0000075077105,0.000047823076,0.0022522027,0.00025306802,0.00045725523,0.0045441436,0.00018272869,0.0034824796,0.000025582376],"about_ca_topic_score_codex":0.0060095545,"about_ca_topic_score_gemma":0.017937234,"teacher_disagreement_score":0.0060095545,"about_ca_system_score_codex":0.00054741115,"about_ca_system_score_gemma":0.0003443461,"threshold_uncertainty_score":0.011949122},"labels":[],"label_agreement":null},{"id":"W2029515740","doi":"10.1086/502648","title":"Discovery of the X-Ray Counterpart to the Rotating Radio Transient J1819-1458","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Neutron star; Pulsar; Black-body radiation; Transient (computer programming); Position (finance); Position angle; Infrared; Pulse (music); Flux (metallurgy)","score_opus":0.007282691619073897,"score_gpt":0.2751268148434924,"score_spread":0.2678441232244185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029515740","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99523926,0.00042883906,0.00055704336,0.00007325413,0.000042453124,0.0000132545365,0.0001786687,0.00004883995,0.0034183967],"genre_scores_gemma":[0.9965037,0.000248978,0.0013330902,0.00010571005,0.00010339915,0.000012546408,0.0007329294,0.000015745052,0.00094398134],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999275,0.0000028410288,0.0000044836415,0.000027664002,0.000016817161,0.000020640768],"domain_scores_gemma":[0.99976104,0.000014905039,0.00010028902,0.000024366465,0.00002557566,0.00007385898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011321613,0.00020166319,0.00022446453,0.0006408817,0.00041390874,0.00086620764,0.0004573168,0.000459563,0.0014546667],"category_scores_gemma":[0.00025561888,0.00013045533,0.00016217983,0.0003549564,0.0002889159,0.00031970793,0.0006832813,0.00031238224,0.000637577],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007147484,0.00027900632,0.38475603,0.0002450175,0.00016124026,0.01842579,0.0009686246,0.00040132774,0.51949644,0.004370649,0.0022632543,0.06791799],"study_design_scores_gemma":[0.00008388089,0.000884335,0.90577424,0.000054087526,0.00013562066,0.018174771,0.0003158572,0.001248313,0.030626127,0.00064080965,0.042020436,0.000041578653],"about_ca_topic_score_codex":0.00043683566,"about_ca_topic_score_gemma":0.00051650166,"teacher_disagreement_score":0.0014546667,"about_ca_system_score_codex":0.0001878739,"about_ca_system_score_gemma":0.000096297255,"threshold_uncertainty_score":0.004866421},"labels":[],"label_agreement":null},{"id":"W2029543954","doi":"10.1086/318905","title":"Supernova 1991T and the Value of the Hubble Constant","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Hubble's law; Supernova; Hubble space telescope; Luminosity; Metallicity; Cosmic distance ladder; Hubble Deep Field","score_opus":0.008083525159412684,"score_gpt":0.21553503046960013,"score_spread":0.20745150531018744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029543954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993739,0.0007755985,0.0021350717,0.000035894445,0.000006418039,0.000008629797,0.00043745906,0.00004092653,0.0028209162],"genre_scores_gemma":[0.99869835,0.00021806626,0.00040687842,0.000005343523,0.000007983755,0.0000030451993,0.00040121606,0.00000475748,0.00025426637],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998342,0.000022656957,0.00001339664,0.000063682295,0.00003957308,0.0000265558],"domain_scores_gemma":[0.9971512,0.00058250205,0.0015445988,0.00032315918,0.00016821525,0.00023035711],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042274134,0.00025862386,0.00018497654,0.0007987333,0.00020142319,0.0005001234,0.0002933885,0.00014193835,0.0014039463],"category_scores_gemma":[0.0036032381,0.000108820714,0.00011908306,0.0006596115,0.00060550525,0.0002464217,0.00040748337,0.00025931667,0.00048086754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060912138,0.00000823283,0.98656,0.000018295474,0.000057920028,0.0001476865,0.000062702195,0.0018091338,0.003123181,0.001652146,0.00019111486,0.0063088154],"study_design_scores_gemma":[0.0000038049893,0.000022386293,0.99381953,0.000006402505,0.000022085283,0.0005651409,0.000030962987,0.0018066866,0.0017022152,0.0006033183,0.0014101971,0.0000072229427],"about_ca_topic_score_codex":0.0062534404,"about_ca_topic_score_gemma":0.004639531,"teacher_disagreement_score":0.0062534404,"about_ca_system_score_codex":0.0005204458,"about_ca_system_score_gemma":0.00030818142,"threshold_uncertainty_score":0.012434125},"labels":[],"label_agreement":null},{"id":"W2029664173","doi":"10.1088/0004-637x/714/2/1037","title":"A SPECTROSCOPIC ANALYSIS OF WHITE DWARFS IN THE KISO SURVEY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Stars; Physics; White dwarf; Astrophysics; Luminosity function; Luminosity; Degenerate energy levels; Astronomy; Galaxy","score_opus":0.011648584071043093,"score_gpt":0.24826316771885087,"score_spread":0.23661458364780777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029664173","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978896,0.00011982189,0.00019519901,0.000019191,0.0000015883649,0.0000057987986,0.00053716556,0.000012169505,0.0012194909],"genre_scores_gemma":[0.99715483,0.00018150869,0.00056997826,0.000019012907,0.0000056486674,0.0000069815624,0.0014812048,0.000005348448,0.00057528476],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985397,0.000012142054,0.000012476289,0.000037829188,0.00004289005,0.000040650568],"domain_scores_gemma":[0.9995516,0.00003084185,0.00013064698,0.000040748804,0.0001355201,0.00011068215],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001433003,0.00020857123,0.00014704693,0.0031152542,0.0004148999,0.00031550307,0.00014407291,0.0001294821,0.00084168976],"category_scores_gemma":[0.00047378318,0.00010879655,0.00013429305,0.001821699,0.0001790324,0.00021359001,0.0005876995,0.000116028605,0.0004273474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046194524,0.000024259836,0.9771906,0.000026748447,0.000019316467,0.0001339728,0.0004954761,0.0000967945,0.01153501,0.00013806533,0.00026419744,0.010029363],"study_design_scores_gemma":[8.011871e-7,0.000015592512,0.9986897,0.0000022822785,0.0000046282407,0.000100583435,0.00016026579,0.00007421085,0.00021188885,0.000018734296,0.0007200068,0.0000013797116],"about_ca_topic_score_codex":0.011259999,"about_ca_topic_score_gemma":0.02156364,"teacher_disagreement_score":0.011259999,"about_ca_system_score_codex":0.00025841754,"about_ca_system_score_gemma":0.00027867532,"threshold_uncertainty_score":0.022388935},"labels":[],"label_agreement":null},{"id":"W2029740442","doi":"10.1088/0004-637x/702/1/l61","title":"SUBDEGREE SUNYAEV-ZEL'DOVICH SIGNAL FROM MULTIFREQUENCY BOOMERANG OBSERVATIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council; National Science Foundation","keywords":"Cosmic microwave background; Physics; Sunyaev–Zel'dovich effect; CMB cold spot; Astrophysics; Cosmic background radiation; Anisotropy; Compton scattering; Background radiation; Planck; Computational physics; Photon; Nuclear physics; Optics; Radiation","score_opus":0.018332267375488362,"score_gpt":0.25135815363392355,"score_spread":0.23302588625843518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029740442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954377,0.00011080079,0.0017057788,0.00008261554,0.000004653388,0.0000057480906,0.0003825107,0.000056747696,0.0022134339],"genre_scores_gemma":[0.9984989,0.000047004578,0.0006053674,0.000015724409,0.000004163781,0.0000027686494,0.0006383874,0.000013993531,0.00017369227],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970645,0.000062040264,0.000009684325,0.00007129101,0.00008407355,0.00006652991],"domain_scores_gemma":[0.99952316,0.00011135967,0.00017935035,0.00007063225,0.000042931017,0.00007260285],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050907326,0.0003326921,0.00032031632,0.00067285827,0.0002798484,0.00068045186,0.00024651497,0.00016253852,0.0008759296],"category_scores_gemma":[0.001301108,0.00016710372,0.00025627165,0.00052506657,0.0004007675,0.00023595127,0.00078349555,0.00025848974,0.00013761093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058441126,0.000035217126,0.920385,0.00009958549,0.00024076823,0.000319977,0.0004582156,0.0131846275,0.024525702,0.0039621214,0.0011844813,0.035019856],"study_design_scores_gemma":[0.000022899734,0.000021089869,0.9826843,0.000013157613,0.000043765867,0.00007814269,0.00005069711,0.011041857,0.0030496733,0.0006858867,0.0022906759,0.000017837257],"about_ca_topic_score_codex":0.022137156,"about_ca_topic_score_gemma":0.051093247,"teacher_disagreement_score":0.022137156,"about_ca_system_score_codex":0.00059244875,"about_ca_system_score_gemma":0.0003218772,"threshold_uncertainty_score":0.0440166},"labels":[],"label_agreement":null},{"id":"W2029775612","doi":"10.1088/0004-637x/707/1/310","title":"OUTFLOWS AND MASSIVE STARS IN THE PROTOCLUSTER IRAS 05358+3543","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"James Clerk Maxwell Telescope; Stars; Observatory; Telescope; Spectral line; Line-of-sight; Point source; Star formation; Line (geometry)","score_opus":0.010296772277312113,"score_gpt":0.24781544989312299,"score_spread":0.23751867761581086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029775612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996371,0.000036243247,0.00004293509,0.00000539815,6.9413466e-7,7.955456e-7,0.000015303109,0.000005134281,0.00025633548],"genre_scores_gemma":[0.99962246,0.000027616581,0.00014891317,0.0000096703425,0.000001820811,8.280325e-7,0.00006974396,0.0000011270148,0.00011783148],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999273,0.000005648249,0.0000049965365,0.00001459451,0.000024388048,0.000023021823],"domain_scores_gemma":[0.9998036,0.000012583177,0.000089399255,0.000013094845,0.000016653017,0.00006468601],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011379519,0.00014450657,0.000093502786,0.00051028735,0.00042816252,0.0002892568,0.00019564299,0.00016100112,0.0004923243],"category_scores_gemma":[0.00023549233,0.0000983223,0.0001045721,0.00033615803,0.0002456148,0.0001852632,0.00036000062,0.00012604585,0.00012234176],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008711186,0.000034861612,0.95204395,0.000016734744,0.000022644657,0.0009797122,0.0005965416,0.00034533575,0.034808192,0.0002745425,0.00019110779,0.010599218],"study_design_scores_gemma":[0.0000035767966,0.000048391586,0.9968839,0.0000037190957,0.0000091061165,0.00064975914,0.0001143406,0.00038063008,0.0011695414,0.0000872259,0.0006458781,0.0000039626057],"about_ca_topic_score_codex":0.005899533,"about_ca_topic_score_gemma":0.014934839,"teacher_disagreement_score":0.005899533,"about_ca_system_score_codex":0.00022976505,"about_ca_system_score_gemma":0.00013670472,"threshold_uncertainty_score":0.011730373},"labels":[],"label_agreement":null},{"id":"W2029784035","doi":"10.1086/374217","title":"Nuclear Composition of Gamma‐Ray Burst Fireballs","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":198,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Gamma-ray burst; Nucleosynthesis; Spallation; Nuclear physics; Neutron; Afterglow; Neutrino; Astrophysics; Neutron emission; Deuterium; Observable; Nucleon; Neutron star; Nuclear reaction; Neutron temperature","score_opus":0.008558317220003166,"score_gpt":0.2162996513119468,"score_spread":0.20774133409194365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029784035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962392,0.00045593595,0.0015014103,0.000017142456,0.000010895036,0.000008071871,0.00007621896,0.000016487344,0.0016746152],"genre_scores_gemma":[0.9976483,0.00045524992,0.0007506361,0.000012262852,0.000008698484,0.000010035218,0.00031250223,0.000021060183,0.0007813484],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998572,0.00001925018,0.000009963422,0.000041453095,0.000032147604,0.000039841147],"domain_scores_gemma":[0.9995789,0.00008418645,0.00017000454,0.00003392544,0.00006081502,0.00007214748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052556256,0.000379437,0.00038442985,0.0014832669,0.00052022113,0.0014247254,0.00038390854,0.00031649304,0.00094065256],"category_scores_gemma":[0.0010877465,0.00025158754,0.0003465523,0.0005323206,0.0005673279,0.00037525824,0.00059226074,0.00024077256,0.0002507599],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023162938,0.00018240444,0.28412485,0.00024436292,0.00030083192,0.002415272,0.00083259994,0.039984718,0.6127127,0.027070839,0.0006123665,0.029202754],"study_design_scores_gemma":[0.0002696235,0.0011005509,0.37877506,0.00019845027,0.00045406664,0.006198018,0.0013854069,0.22235866,0.34989503,0.028239261,0.010938701,0.00018718105],"about_ca_topic_score_codex":0.0017824934,"about_ca_topic_score_gemma":0.0009849867,"teacher_disagreement_score":0.0017824934,"about_ca_system_score_codex":0.0005946689,"about_ca_system_score_gemma":0.00020307736,"threshold_uncertainty_score":0.0043147206},"labels":[],"label_agreement":null},{"id":"W2029795678","doi":"10.1086/321416","title":"LB 8827: A Variable, Magnetic DBA White Dwarf","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; White dwarf; Balmer series; Brightness; Spectral line; Stars; Amplitude; Magnetic field; Circular polarization; Spectral energy distribution; Cataclysmic variable star; RADIUS; Astronomy; Emission spectrum; Optics","score_opus":0.008335603325826486,"score_gpt":0.2084932214395492,"score_spread":0.20015761811372274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029795678","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99658716,0.00008255191,0.00012637413,0.000033017062,0.0000055196783,0.0000054745515,0.00042082302,0.000028044422,0.0027110926],"genre_scores_gemma":[0.9970331,0.00005763245,0.00041194816,0.00004197631,0.000007834281,0.000005439896,0.0012283296,0.000012732164,0.0012009287],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999356,0.0000026377897,0.0000038075711,0.000016592798,0.000021671822,0.000019628644],"domain_scores_gemma":[0.9998822,0.0000039655433,0.000032356205,0.000012638023,0.000014605547,0.000054215707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000055813078,0.00030261342,0.00023157844,0.0006590004,0.00050086074,0.0003307469,0.00031668195,0.00019712525,0.00080098334],"category_scores_gemma":[0.0001110842,0.000106669155,0.0000636746,0.0004740414,0.00029803318,0.00012962872,0.00035000054,0.0002336978,0.0011778993],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050830597,0.00035771585,0.73749226,0.00009692884,0.000049181566,0.004500317,0.0007227585,0.00036552348,0.2210891,0.0009440492,0.0050491816,0.028824696],"study_design_scores_gemma":[0.000045341294,0.00045647455,0.9465219,0.000017887303,0.0000350603,0.009193582,0.00067790033,0.0011337412,0.018047728,0.00029503007,0.023556542,0.000018769793],"about_ca_topic_score_codex":0.005592343,"about_ca_topic_score_gemma":0.008451311,"teacher_disagreement_score":0.005592343,"about_ca_system_score_codex":0.00035973493,"about_ca_system_score_gemma":0.00013632176,"threshold_uncertainty_score":0.011119604},"labels":[],"label_agreement":null},{"id":"W2029854188","doi":"10.1086/339426","title":"The Las Campanas Infrared Survey. III. The<i>H</i>‐Band Imaging Survey and the Near‐Infrared and Optical Photometric Catalogs","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Raymond and Beverly Sackler Foundation; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Sky; Photometry (optics); Infrared; Redshift; Luminous infrared galaxy; Astronomy","score_opus":0.010450249179015188,"score_gpt":0.21008768327132854,"score_spread":0.19963743409231335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2029854188","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2914351,0.014301691,0.00621602,0.0061899116,0.0009852262,0.00265295,0.34008354,0.003508282,0.33462727],"genre_scores_gemma":[0.35955504,0.006841977,0.02463175,0.0059972373,0.0011882782,0.004075559,0.4348217,0.00068806385,0.16220038],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99936014,0.000052256728,0.000025398576,0.0001628082,0.00025838646,0.00014104931],"domain_scores_gemma":[0.99904734,0.000054150085,0.00019015712,0.00010154594,0.00043009786,0.00017671478],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008612732,0.000622194,0.0003964743,0.002576712,0.0007856641,0.0013722909,0.0009175508,0.00041495802,0.00865755],"category_scores_gemma":[0.00069721066,0.00031110927,0.00024576308,0.0029446224,0.0003063286,0.00050049997,0.0010954656,0.00082311034,0.0047032647],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041697436,0.00034064928,0.24199595,0.00090666313,0.00015482603,0.00038779314,0.00058190664,0.0004918301,0.008120343,0.005881871,0.50971466,0.23100649],"study_design_scores_gemma":[0.00010418961,0.000042456606,0.6199497,0.00033148227,0.000038837356,0.00018542922,0.00046437592,0.00046178358,0.0010121113,0.0007513136,0.3766354,0.000022886588],"about_ca_topic_score_codex":0.10956216,"about_ca_topic_score_gemma":0.11151295,"teacher_disagreement_score":0.10956216,"about_ca_system_score_codex":0.0014464243,"about_ca_system_score_gemma":0.0018216121,"threshold_uncertainty_score":0.2178489},"labels":[],"label_agreement":null},{"id":"W2030094391","doi":"10.1088/0004-637x/716/1/556","title":"ULTRAVIOLET+INFRARED STAR FORMATION RATES: HICKSON COMPACT GROUPS WITH<i>SWIFT</i>AND<i>SPITZER</i>","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Astrophysics; Physics; Galaxy; Star formation; Photometry (optics); Bimodality; Astronomy; Stars","score_opus":0.005654855623513789,"score_gpt":0.20503762261075242,"score_spread":0.19938276698723864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030094391","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987871,0.000056971065,0.000060844202,0.0000067901697,9.655338e-7,0.000003915424,0.0003697881,0.000007738454,0.0007058791],"genre_scores_gemma":[0.9989343,0.000015770713,0.000080935504,0.0000038455432,0.0000030070125,0.0000026771029,0.0007546642,0.000002049961,0.00020275862],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987125,0.000010977534,0.000008245562,0.000044566714,0.000029187371,0.00003576367],"domain_scores_gemma":[0.99948645,0.000037190828,0.00025922156,0.000039310653,0.00006148479,0.00011632719],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022179037,0.00022159147,0.00014005839,0.001431443,0.00013728955,0.00035239896,0.00019245893,0.00016265124,0.0015324587],"category_scores_gemma":[0.0005533651,0.00007614778,0.00016378173,0.0006854031,0.00021444625,0.0003411345,0.00043073425,0.00012872707,0.0002969186],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006103205,0.000017488277,0.9956709,0.000005931079,0.000024503332,0.000030154075,0.0000916377,0.00020574093,0.0011381152,0.000056835037,0.00015229412,0.0025454068],"study_design_scores_gemma":[0.0000012051389,0.000022315207,0.99939287,0.0000015099332,0.0000066003527,0.000044400258,0.000039177783,0.00017953129,0.00016357488,0.000017742503,0.00012986753,0.0000011409123],"about_ca_topic_score_codex":0.0063807736,"about_ca_topic_score_gemma":0.0073458333,"teacher_disagreement_score":0.0063807736,"about_ca_system_score_codex":0.00021621604,"about_ca_system_score_gemma":0.00006482187,"threshold_uncertainty_score":0.012687266},"labels":[],"label_agreement":null},{"id":"W2030115818","doi":"10.1088/0004-637x/754/2/143","title":"MAGNIFICATION BY GALAXY GROUP DARK MATTER HALOS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Magnification; Dark matter; Galaxy; Gravitational lens; Weak gravitational lensing; Strong gravitational lensing; Halo; Consistency (knowledge bases)","score_opus":0.006395454252255519,"score_gpt":0.2040818913219544,"score_spread":0.19768643706969888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030115818","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960601,0.00020573479,0.0027572752,0.000020269985,0.0000031380202,0.0000069935313,0.000093320836,0.000056890392,0.00079636247],"genre_scores_gemma":[0.9991227,0.00003381163,0.0006871277,0.000003851264,0.000005754226,0.0000014724545,0.000086194654,0.0000054421084,0.00005366299],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99931467,0.00018179795,0.00002847845,0.00019257,0.00018945057,0.000093035196],"domain_scores_gemma":[0.9937216,0.0023786882,0.0022450504,0.00083192,0.00038185145,0.00044097824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016834193,0.0006016487,0.0003315649,0.0021041557,0.0002823502,0.0007087171,0.00044836325,0.00026456732,0.0009620728],"category_scores_gemma":[0.0070302095,0.00024937134,0.00047740858,0.0010855685,0.00068785145,0.00046922648,0.0009817587,0.00024641652,0.00012975647],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002619459,0.000026985079,0.9564225,0.0000564603,0.0002563613,0.00021342997,0.00034668864,0.0076010856,0.017279388,0.0018827883,0.00020172773,0.015450698],"study_design_scores_gemma":[0.000015430156,0.00013650996,0.95317054,0.000013200114,0.0001233193,0.00043337492,0.00011260562,0.030856652,0.011288137,0.00295756,0.00085187546,0.00004081372],"about_ca_topic_score_codex":0.0020071503,"about_ca_topic_score_gemma":0.0015658485,"teacher_disagreement_score":0.0021041557,"about_ca_system_score_codex":0.00046674552,"about_ca_system_score_gemma":0.00012929887,"threshold_uncertainty_score":0.008902848},"labels":[],"label_agreement":null},{"id":"W2030156602","doi":"10.1088/0004-637x/745/1/86","title":"STELLAR POPULATIONS OF HIGHLY MAGNIFIED LENSED GALAXIES: YOUNG STARBURSTS AT<i>z</i>∼ 2","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Galaxy; Stellar population; Star formation; Photometry (optics); Extinction (optical mineralogy); Luminosity; Population; Luminous infrared galaxy","score_opus":0.015014391656660082,"score_gpt":0.2263227300031949,"score_spread":0.2113083383465348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030156602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997336,0.0003733573,0.00012738905,0.00001329213,9.1623104e-7,0.000004206596,0.0009336413,0.000026072945,0.0011850672],"genre_scores_gemma":[0.9966348,0.0002813678,0.00024039505,0.000012587057,0.0000060819225,0.0000029544856,0.0023953016,0.00000882531,0.00041785176],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998777,0.000007249128,0.000013246773,0.000039482627,0.000031567073,0.00003076609],"domain_scores_gemma":[0.9992899,0.00007685281,0.00035859252,0.000057880134,0.00009096137,0.00012581192],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021835383,0.00021746603,0.0002470778,0.0032291154,0.00023892387,0.0007753352,0.00025701625,0.00015711084,0.0010827958],"category_scores_gemma":[0.000530788,0.00011969646,0.00019400031,0.0022601192,0.00025346116,0.00037886357,0.00044788886,0.00012613338,0.00036306548],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043950167,0.000010636753,0.98918086,0.000023561719,0.00003865863,0.00014351403,0.00036127312,0.0001378585,0.0028761746,0.00009216406,0.00019595174,0.006895236],"study_design_scores_gemma":[8.341532e-7,0.000008407801,0.9989919,0.0000031341797,0.0000120112845,0.00015300038,0.000090588546,0.00006990106,0.0002605873,0.000024020106,0.00038383913,0.0000017167469],"about_ca_topic_score_codex":0.0124805635,"about_ca_topic_score_gemma":0.022708358,"teacher_disagreement_score":0.0124805635,"about_ca_system_score_codex":0.00036934623,"about_ca_system_score_gemma":0.00016895037,"threshold_uncertainty_score":0.024815798},"labels":[],"label_agreement":null},{"id":"W2030198327","doi":"10.1088/0004-637x/798/2/73","title":"BANYAN. V. A SYSTEMATIC ALL-SKY SURVEY FOR NEW VERY LATE-TYPE LOW-MASS STARS AND BROWN DWARFS IN NEARBY YOUNG MOVING GROUPS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Proper motion; Stars; Stellar classification; Exoplanet; Sky; Galactic plane","score_opus":0.014696611562206916,"score_gpt":0.22622800825852749,"score_spread":0.21153139669632057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030198327","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89829266,0.0011860871,0.008755714,0.00015566775,0.00007145854,0.00040171118,0.059922904,0.0014490732,0.029764798],"genre_scores_gemma":[0.76504153,0.0009830139,0.042543117,0.00019606885,0.00014341749,0.0007162591,0.1674766,0.0005012567,0.022398748],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997104,0.000036129564,0.000019412766,0.00008799354,0.00008823168,0.00005781863],"domain_scores_gemma":[0.9987226,0.00006928247,0.00036750597,0.00020435407,0.00022874308,0.00040747153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006408008,0.00033430185,0.0002824283,0.0024190224,0.0007610509,0.00057929306,0.00045264515,0.00014950459,0.003557411],"category_scores_gemma":[0.0006120597,0.00024598202,0.00014911634,0.0016131971,0.00014589804,0.00036256414,0.0010921083,0.00026464503,0.0018285731],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033405932,0.000120910525,0.8829806,0.00019348,0.00007465368,0.00020938419,0.0006267111,0.00032603563,0.018674914,0.0010261695,0.016523188,0.078909844],"study_design_scores_gemma":[0.000029026152,0.00005259011,0.94622594,0.000027147827,0.00003110962,0.0003525768,0.00022297072,0.0005693159,0.0027530044,0.00027307507,0.049450673,0.000012569421],"about_ca_topic_score_codex":0.016957562,"about_ca_topic_score_gemma":0.026687201,"teacher_disagreement_score":0.016957562,"about_ca_system_score_codex":0.00026870126,"about_ca_system_score_gemma":0.00096586585,"threshold_uncertainty_score":0.033717692},"labels":[],"label_agreement":null},{"id":"W2030433459","doi":"10.1086/510114","title":"A Search for Nitrogen‐enhanced Metal‐poor Stars","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Physics; Astrophysics; Asymptotic giant branch; K-type main-sequence star; Carbon fibers; Nitrogen; Metal; T Tauri star; Chemistry; Materials science; Composite material; Organic chemistry","score_opus":0.017575745641117312,"score_gpt":0.2654669031538292,"score_spread":0.2478911575127119,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030433459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99773943,0.0003984188,0.00038295795,0.00007233863,0.000004311724,0.000011410987,0.000115865005,0.00001931975,0.0012559955],"genre_scores_gemma":[0.9979874,0.00018122488,0.00081917987,0.00014443754,0.000026693555,0.000009584693,0.00045737525,0.000007457529,0.00036665297],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994074,0.00004727939,0.000045851597,0.00024618625,0.00016836208,0.000084965286],"domain_scores_gemma":[0.9984011,0.00022670953,0.0005530654,0.00015415653,0.00018981821,0.00047509052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007150406,0.00040497843,0.00054265803,0.0019871215,0.0012042875,0.0010369315,0.0007487872,0.00089773495,0.0014715944],"category_scores_gemma":[0.0009116009,0.00023896125,0.00024267042,0.0014574733,0.00063167705,0.000638974,0.00088483014,0.00041001415,0.0008608482],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002778148,0.00009716161,0.9358408,0.00008710125,0.00009538635,0.00078103313,0.00029725127,0.00022539534,0.04758538,0.0003756252,0.00034927813,0.013987844],"study_design_scores_gemma":[0.000021954553,0.00021883118,0.986485,0.000019536395,0.000059203456,0.002169918,0.00028428473,0.00073036476,0.007289897,0.00042611815,0.002282513,0.000012416998],"about_ca_topic_score_codex":0.00064694707,"about_ca_topic_score_gemma":0.0010940895,"teacher_disagreement_score":0.0019871215,"about_ca_system_score_codex":0.000283241,"about_ca_system_score_gemma":0.00042632877,"threshold_uncertainty_score":0.0049230456},"labels":[],"label_agreement":null},{"id":"W2030441303","doi":"10.1086/588274","title":"Self‐organized Critical Model of Energy Release in an Idealized Coronal Loop","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Coronal loop; Solar flare; Flare; Magnetic reconnection; Anisotropy; Magnetic flux; Astrophysics; Geometry; Statistical physics; Magnetic field; Coronal mass ejection; Solar wind; Optics","score_opus":0.012495951547645708,"score_gpt":0.24281756710575667,"score_spread":0.23032161555811095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030441303","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.69500655,0.0005102124,0.27601334,0.00090832147,0.00012017191,0.00007668788,0.00025774582,0.00027443873,0.026832592],"genre_scores_gemma":[0.99144673,0.000110172645,0.00474551,0.000047171674,0.000021367028,0.000064418375,0.00004558451,0.000018259252,0.0035008355],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984396,0.000034169487,0.000007205379,0.000031341242,0.00003894114,0.0000443532],"domain_scores_gemma":[0.9996587,0.00009325415,0.00007887222,0.000038426424,0.00005334034,0.000077327815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027549992,0.0003591493,0.00054709014,0.0005579766,0.0006635212,0.0012126409,0.001147042,0.0008596564,0.002472522],"category_scores_gemma":[0.000866804,0.00023257858,0.0006158266,0.00026295663,0.0016832359,0.001242812,0.0007413392,0.0005422054,0.00018307587],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008899302,0.00004776873,0.0009854261,0.000036307836,0.000037134203,0.00033403607,0.00019847004,0.7656331,0.005475632,0.22480619,0.0005807542,0.0017761554],"study_design_scores_gemma":[0.000026393118,0.000030024,0.00016607884,0.0000029997514,0.000006077988,0.000038902293,0.00003092821,0.962844,0.00021480313,0.036161482,0.0004687322,0.00000961631],"about_ca_topic_score_codex":0.0033124667,"about_ca_topic_score_gemma":0.0011744715,"teacher_disagreement_score":0.0033124667,"about_ca_system_score_codex":0.00095966825,"about_ca_system_score_gemma":0.0006217032,"threshold_uncertainty_score":0.008271396},"labels":[],"label_agreement":null},{"id":"W2030589003","doi":"10.1086/338838","title":"Discriminating Weak Lensing from Intrinsic Spin Correlations Using the Curl‐Gradient Decomposition","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":250,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Curl (programming language); Physics; Cosmic microwave background; Weak gravitational lensing; Redshift; Polarization (electrochemistry); Distortion (music); Galaxy; Cosmology; Astrophysics; Optics; Computer science; Anisotropy","score_opus":0.017709313358273537,"score_gpt":0.24196401278373633,"score_spread":0.2242546994254628,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030589003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7390996,0.00030206822,0.2555779,0.0004363928,0.000025644229,0.000053066746,0.0007851281,0.00063567935,0.00308455],"genre_scores_gemma":[0.9488575,0.00020124143,0.049244527,0.000045507615,0.0000524868,0.000031260883,0.00082664454,0.000086652304,0.00065409363],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99952483,0.00014748523,0.000031884574,0.00008215203,0.00014594544,0.00006760394],"domain_scores_gemma":[0.99709284,0.0010461875,0.00072481117,0.00049954007,0.0003318641,0.00030467391],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012186419,0.0005871626,0.00047464677,0.0018381526,0.0002957667,0.00135253,0.0002531185,0.0002878307,0.0008981122],"category_scores_gemma":[0.005215656,0.00026188052,0.00027561423,0.0009474936,0.0007950444,0.0007881446,0.0009901649,0.00050374406,0.00031027902],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010474275,0.0001933443,0.15425584,0.00031388595,0.0004240672,0.0005943089,0.0008394738,0.06309123,0.2953039,0.075159855,0.00503485,0.4037418],"study_design_scores_gemma":[0.000102877435,0.00017198424,0.2209204,0.000041796677,0.00012662905,0.00059371325,0.00029254807,0.61108977,0.056143392,0.10393258,0.0063652205,0.00021908183],"about_ca_topic_score_codex":0.001606209,"about_ca_topic_score_gemma":0.0023924285,"teacher_disagreement_score":0.0018381526,"about_ca_system_score_codex":0.0004158177,"about_ca_system_score_gemma":0.0004964065,"threshold_uncertainty_score":0.0064448714},"labels":[],"label_agreement":null},{"id":"W2030622210","doi":"10.1088/0004-637x/739/1/39","title":"DISCOVERY OF AN ENERGETIC PULSAR ASSOCIATED WITH SNR G76.9+1.0","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Manitoba","funders":"","keywords":"Pulsar; Vela; Supernova remnant; Luminosity; Millisecond pulsar; Supernova; Neutron star; Magnetic dipole; Interstellar medium","score_opus":0.016254562485102788,"score_gpt":0.2782027955643069,"score_spread":0.2619482330792041,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030622210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99844813,0.00015725417,0.000107490116,0.000031142397,0.000014415371,0.0000059047265,0.00007999788,0.000018182238,0.0011374855],"genre_scores_gemma":[0.9981036,0.00015140824,0.0005679404,0.00008066462,0.000027166565,0.0000058783203,0.00037178054,0.000004653692,0.0006868401],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993145,0.00000362484,0.0000055156893,0.000016631604,0.000020810814,0.00002198322],"domain_scores_gemma":[0.99984705,0.000009206098,0.000051702416,0.000019729503,0.00001526613,0.000057015593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000131228,0.00030983117,0.00023786991,0.0004479559,0.000584731,0.00055427063,0.0002251354,0.00046115948,0.00089251355],"category_scores_gemma":[0.00031402605,0.000132396,0.00010461758,0.00031970826,0.00028916114,0.00021141335,0.0006863265,0.00022228915,0.0006398073],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012284818,0.00019204109,0.37063697,0.0001572469,0.000090337635,0.020541158,0.00068812416,0.00054298766,0.57112175,0.0012936672,0.0009006551,0.032606617],"study_design_scores_gemma":[0.00007115534,0.0017060287,0.8804631,0.000040716637,0.00011262452,0.037938837,0.0005462828,0.0008175473,0.06118077,0.0009936747,0.016085632,0.0000435584],"about_ca_topic_score_codex":0.0007446297,"about_ca_topic_score_gemma":0.0012320264,"teacher_disagreement_score":0.00089251355,"about_ca_system_score_codex":0.00017647973,"about_ca_system_score_gemma":0.00012553547,"threshold_uncertainty_score":0.0029857755},"labels":[],"label_agreement":null},{"id":"W2030627151","doi":"10.1088/0004-637x/700/1/1","title":"THE<i>CHANDRA</i>DEEP PROTOCLUSTER SURVEY: Lyα BLOBS ARE POWERED BY HEATING, NOT COOLING","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leverhulme Trust; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Science and Technology Facilities Council; Smithsonian Institution","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Luminosity; Flux (metallurgy); Photoionization; Infrared; Astronomy; Ionization; Ion","score_opus":0.008744984838373868,"score_gpt":0.22425362007338875,"score_spread":0.2155086352350149,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030627151","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968426,0.0002838459,0.0003749624,0.00003415247,0.0000035660698,0.0000066220086,0.0009556673,0.00005562648,0.00144304],"genre_scores_gemma":[0.9974254,0.0002308291,0.0007369686,0.00004849782,0.0000134406455,0.000005040838,0.0011708637,0.000016639899,0.00035226313],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988127,0.000007095186,0.0000063192315,0.00003743005,0.000032085005,0.000035763827],"domain_scores_gemma":[0.9994696,0.00004237003,0.00022387168,0.000053650812,0.00006538591,0.00014509309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013470332,0.00026314572,0.00021218944,0.00092818233,0.00028201443,0.0006093935,0.0002505737,0.000120668046,0.00093095406],"category_scores_gemma":[0.00039144725,0.00011132596,0.00013510996,0.0008514556,0.00031854786,0.00037813652,0.0005288747,0.00019030369,0.00032264594],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017456415,0.00001907243,0.9546918,0.00004018963,0.00006887931,0.00019740983,0.00020429275,0.00022921023,0.030824987,0.0002037431,0.0009982919,0.012347479],"study_design_scores_gemma":[0.00000347827,0.000022208838,0.99664587,0.0000039164456,0.000013754017,0.00022566979,0.00007195286,0.00018846142,0.0017502723,0.000046906203,0.0010233335,0.0000040789423],"about_ca_topic_score_codex":0.008553538,"about_ca_topic_score_gemma":0.020155223,"teacher_disagreement_score":0.008553538,"about_ca_system_score_codex":0.00025289005,"about_ca_system_score_gemma":0.0001817221,"threshold_uncertainty_score":0.01700747},"labels":[],"label_agreement":null},{"id":"W2030663701","doi":"10.1088/0004-637x/783/2/121","title":"BANYAN. II. VERY LOW MASS AND SUBSTELLAR CANDIDATE MEMBERS TO NEARBY, YOUNG KINEMATIC GROUPS WITH PREVIOUSLY KNOWN SIGNS OF YOUTH","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":302,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Parallax; Proper motion; Bayesian probability; Kinematics; Astrophysics; Sky; Stars; Outlier; Physics; Artificial intelligence; Computer science; Astronomy","score_opus":0.00620322648359843,"score_gpt":0.19477155669780727,"score_spread":0.18856833021420885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030663701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7989094,0.0008803021,0.18373245,0.00020240327,0.00003150244,0.0002485719,0.004101192,0.001135577,0.010758561],"genre_scores_gemma":[0.9207797,0.00020969588,0.068844855,0.00007684403,0.000036320504,0.00011627096,0.0060852384,0.00015428803,0.0036968302],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99913967,0.00015670057,0.000058425867,0.00026013417,0.00025567433,0.00012922466],"domain_scores_gemma":[0.9977489,0.00057698286,0.00074383366,0.00022274836,0.00047521052,0.00023230321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023319742,0.00045341344,0.0004903818,0.002432654,0.0010020589,0.0015796361,0.00086592074,0.00039536293,0.0023220112],"category_scores_gemma":[0.005462789,0.0002747953,0.0004380143,0.0012003147,0.00036085673,0.00050047826,0.0013297284,0.00045112657,0.0008164436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026768085,0.00007755066,0.87244976,0.00011881222,0.00023727448,0.0002400581,0.0005986262,0.008945534,0.008832172,0.0044518784,0.0029312973,0.10084932],"study_design_scores_gemma":[0.000039933093,0.000082135084,0.810828,0.000082171595,0.00022385175,0.00082972884,0.00063387264,0.14491726,0.009606893,0.01134227,0.021351052,0.0000629147],"about_ca_topic_score_codex":0.020261196,"about_ca_topic_score_gemma":0.026751634,"teacher_disagreement_score":0.020261196,"about_ca_system_score_codex":0.0007554207,"about_ca_system_score_gemma":0.0012288175,"threshold_uncertainty_score":0.04028654},"labels":[],"label_agreement":null},{"id":"W2030716007","doi":"10.1086/589956","title":"Current Star Formation in the Ophiuchus and Perseus Molecular Clouds: Constraints and Comparisons from Unbiased Submillimeter and Mid‐Infrared Surveys. II.","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Star formation; Current (fluid); Submillimeter Array; James Clerk Maxwell Telescope; Star (game theory)","score_opus":0.02428889396954983,"score_gpt":0.2477865359941778,"score_spread":0.22349764202462796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030716007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99004644,0.0021526194,0.00025097726,0.00021235808,0.00005600012,0.000022813145,0.00311087,0.000020774158,0.0041270875],"genre_scores_gemma":[0.99303037,0.0008058413,0.00039164355,0.00005633611,0.00008854458,0.000011542967,0.0042489753,0.000013042203,0.0013536718],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997311,0.00003123945,0.000029365165,0.000061748724,0.00010303587,0.000043447642],"domain_scores_gemma":[0.99736816,0.0004941774,0.0007538724,0.00017216908,0.0009578244,0.00025377035],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068570965,0.00015166467,0.00020365481,0.0017401619,0.0003400184,0.0009193715,0.00041208882,0.00026875737,0.0036123847],"category_scores_gemma":[0.0036689865,0.00013845619,0.00015348612,0.0012436138,0.00036206315,0.00074673456,0.0005990869,0.00020160993,0.001281574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010890029,0.000018298892,0.9683375,0.00007408197,0.00003092652,0.00008556939,0.00024562763,0.00021063974,0.0017025769,0.00055941206,0.0018728542,0.026753582],"study_design_scores_gemma":[0.0000029118803,0.000009163237,0.9981976,0.000009719403,0.0000059728595,0.000039421928,0.00011294168,0.0000921528,0.00026182784,0.00008781834,0.0011784314,0.0000021302208],"about_ca_topic_score_codex":0.009189859,"about_ca_topic_score_gemma":0.0155339325,"teacher_disagreement_score":0.009189859,"about_ca_system_score_codex":0.00036717084,"about_ca_system_score_gemma":0.00031635456,"threshold_uncertainty_score":0.018272698},"labels":[],"label_agreement":null},{"id":"W2030901478","doi":"10.1088/0004-637x/734/2/89","title":"SIX NEW RECYCLED GLOBULAR CLUSTER PULSARS DISCOVERED WITH THE GREEN BANK TELESCOPE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Globular cluster; Millisecond pulsar; Green Bank Telescope; Luminosity; Pulsar planet; X-ray pulsar; Telescope","score_opus":0.015824482426438937,"score_gpt":0.2728624113689518,"score_spread":0.25703792894251287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030901478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985268,0.00018911768,0.0004679315,0.000038227732,0.00000936751,0.000007807345,0.00021060935,0.000034587854,0.00051550625],"genre_scores_gemma":[0.9953419,0.00022287316,0.002124312,0.000084674146,0.000016966318,0.000014387638,0.001070771,0.0000137272355,0.0011103749],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978894,0.00001657425,0.000012242946,0.000055892022,0.00006925731,0.00005712619],"domain_scores_gemma":[0.9993742,0.00006874999,0.00014005965,0.000090674126,0.000083504245,0.00024276211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003753323,0.00029503644,0.00025868157,0.001066418,0.000705764,0.00079955766,0.00043369268,0.00030839187,0.0006852875],"category_scores_gemma":[0.00056818884,0.0003019333,0.00023514658,0.0008132926,0.00047020992,0.00034106037,0.000805469,0.00048056696,0.00023294141],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025045226,0.00009171203,0.90077573,0.00006307599,0.00011165254,0.0017473393,0.0016973985,0.000480908,0.065687835,0.0007040055,0.0010116711,0.027378308],"study_design_scores_gemma":[0.000040023548,0.00020356305,0.9842823,0.000020329406,0.00006525155,0.0016077698,0.00033029777,0.0010751933,0.00533727,0.00028540447,0.0067237504,0.000028808727],"about_ca_topic_score_codex":0.006660929,"about_ca_topic_score_gemma":0.012141878,"teacher_disagreement_score":0.006660929,"about_ca_system_score_codex":0.00049434986,"about_ca_system_score_gemma":0.00042966966,"threshold_uncertainty_score":0.013244331},"labels":[],"label_agreement":null},{"id":"W2030968793","doi":"10.1088/0004-637x/699/2/1252","title":"THE SIZE, SHAPE, AND ORIENTATION OF COSMOLOGICAL VOIDS IN THE SLOAN DIGITAL SKY SURVEY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Void (composites); Sky; Salient; Redshift; Cosmology; Orientation (vector space); Robustness (evolution)","score_opus":0.009142358435837515,"score_gpt":0.2273066512372586,"score_spread":0.21816429280142108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2030968793","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924345,0.00011395049,0.0036974787,0.00005497541,0.0000028058362,0.000015006454,0.002434063,0.00025081963,0.0009963376],"genre_scores_gemma":[0.99032927,0.000054025855,0.006202394,0.00000831266,0.0000034954624,0.000009350811,0.0031559966,0.000039604718,0.00019750645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996438,0.00008075274,0.00003437501,0.00008300039,0.00009879786,0.0000593276],"domain_scores_gemma":[0.9974147,0.0008700201,0.0007912914,0.0003589242,0.0003318193,0.00023323859],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012183575,0.00015785445,0.00020234117,0.0024043017,0.0004389763,0.0006961633,0.00033832662,0.00021429418,0.00064107106],"category_scores_gemma":[0.0050653717,0.00022325624,0.00028302587,0.0024234152,0.0003922728,0.00044837268,0.0006965638,0.00018267412,0.00016214458],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009993988,0.000027863392,0.95573366,0.000058356996,0.000051663083,0.00009271346,0.00046373447,0.012918236,0.0032682484,0.0016374829,0.0022954398,0.023352709],"study_design_scores_gemma":[0.000010080798,0.000010942164,0.9655973,0.0000116945985,0.000022234903,0.000112156165,0.00019437689,0.029270083,0.0017982281,0.0010535524,0.0018965772,0.000022739712],"about_ca_topic_score_codex":0.026504843,"about_ca_topic_score_gemma":0.041895166,"teacher_disagreement_score":0.026504843,"about_ca_system_score_codex":0.0007662365,"about_ca_system_score_gemma":0.0005301539,"threshold_uncertainty_score":0.052701116},"labels":[],"label_agreement":null},{"id":"W2031013908","doi":"10.1086/309512","title":"The MACHO Project: Microlensing Results from 5.7 Years of Large Magellanic Cloud Observations","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1004,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gravitational microlensing; Physics; Astrophysics; Large Magellanic Cloud; Halo; Galactic halo; Milky Way; Astronomy; Dark matter; Dark matter halo; Gravitational lens; Massive compact halo object; Population; Photometry (optics); Galaxy; Stars; Brown dwarf","score_opus":0.016962021465819998,"score_gpt":0.2370418575508846,"score_spread":0.22007983608506462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031013908","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97312284,0.0012717459,0.0016242557,0.00041173355,0.00006591753,0.000092417205,0.016356792,0.00080665515,0.0062476816],"genre_scores_gemma":[0.9569145,0.00025093366,0.0042264606,0.00016778504,0.00015038905,0.00005742304,0.03550919,0.00018226133,0.0025410473],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996126,0.00003913307,0.000020727834,0.00011526478,0.00011861005,0.00009374652],"domain_scores_gemma":[0.99895954,0.000094227544,0.00022676756,0.00023195289,0.00014664509,0.00034093467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077645684,0.00040975685,0.0003833625,0.0015605103,0.0005774835,0.0011868248,0.00059548364,0.00075638853,0.001177874],"category_scores_gemma":[0.0011102775,0.00028873523,0.0005012455,0.00093253603,0.0003035117,0.0007178635,0.0019401329,0.0006010824,0.0006387715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00295497,0.0010666255,0.775084,0.0003943298,0.0013954589,0.0018305714,0.0016695535,0.003707084,0.05654871,0.0013479425,0.034064863,0.11993596],"study_design_scores_gemma":[0.00010504288,0.00008988144,0.9830015,0.000017759116,0.00012038414,0.0003092377,0.000244181,0.0029701227,0.0022872593,0.00023153232,0.0105862105,0.00003694092],"about_ca_topic_score_codex":0.014382728,"about_ca_topic_score_gemma":0.038573362,"teacher_disagreement_score":0.014382728,"about_ca_system_score_codex":0.00058041746,"about_ca_system_score_gemma":0.00040818902,"threshold_uncertainty_score":0.02859801},"labels":[],"label_agreement":null},{"id":"W2031046569","doi":"10.1088/0004-637x/760/1/90","title":"THE RESPONSE OF GIANT STARS TO DYNAMICAL-TIMESCALE MASS LOSS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Stars; RADIUS; Giant star; Asymptotic giant branch; Red giant; Radiative transfer; Stellar mass loss; Stellar evolution","score_opus":0.008343834864284553,"score_gpt":0.23134243492891715,"score_spread":0.2229986000646326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031046569","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968905,0.00014865356,0.000866046,0.0001338541,0.000015318776,0.000008956589,0.0001287039,0.000073282376,0.0017346311],"genre_scores_gemma":[0.9989742,0.00007556784,0.00037374013,0.000029004977,0.000005426168,0.0000066855255,0.00016009861,0.000027827362,0.00034731996],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999229,0.000013416956,0.0000032597482,0.000016213597,0.000014834047,0.000029473747],"domain_scores_gemma":[0.99959356,0.00012182284,0.000102098966,0.000035869994,0.00005497153,0.00009174341],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002546847,0.00046120034,0.0003762575,0.00030927517,0.00041475415,0.0005892279,0.0005629387,0.0007989613,0.0014527494],"category_scores_gemma":[0.0020660334,0.0002281427,0.0006206837,0.0002298641,0.0004186384,0.0005965465,0.000607547,0.00054755807,0.00028431835],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010392626,0.0003658053,0.13497272,0.0002488267,0.0004918708,0.0010319969,0.00045979198,0.7506679,0.09340235,0.0045250906,0.0016615703,0.011132906],"study_design_scores_gemma":[0.00016720618,0.0006390868,0.082537666,0.00002706104,0.000116667856,0.0002616127,0.00027998508,0.89763767,0.01222597,0.004252059,0.0017930268,0.000061942505],"about_ca_topic_score_codex":0.003810334,"about_ca_topic_score_gemma":0.001754252,"teacher_disagreement_score":0.003810334,"about_ca_system_score_codex":0.0004405387,"about_ca_system_score_gemma":0.00022254598,"threshold_uncertainty_score":0.0075763464},"labels":[],"label_agreement":null},{"id":"W2031068550","doi":"10.1086/321480","title":"Assignment of the λ1369.13 Diffuse Interstellar Absorption Band and Three Other Far‐Ultraviolet Interstellar Absorption Lines to the CH Molecule","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Steacie Institute for Molecular Sciences","funders":"","keywords":"Physics; Interstellar medium; Absorption spectroscopy; Spectral line; Line (geometry); Astrophysics; Astrochemistry; Absorption (acoustics); Ultraviolet; Molecule; Atomic physics; Astronomy; Optics; Galaxy","score_opus":0.010338724980738116,"score_gpt":0.23777303508406572,"score_spread":0.2274343101033276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031068550","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917624,0.000327106,0.0027009202,0.0000888281,0.000014607443,0.00001785234,0.00024350871,0.000055939418,0.004788847],"genre_scores_gemma":[0.9952426,0.00014283841,0.0030202724,0.000050829196,0.000007695351,0.0000148642885,0.0004200245,0.0000073382716,0.0010935479],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.999933,0.000004884727,0.0000028868826,0.000018314102,0.00002205873,0.000018915684],"domain_scores_gemma":[0.99983513,0.000015560647,0.000052931104,0.000010845671,0.000020864249,0.0000646759],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012011746,0.0002763054,0.00014974098,0.000787583,0.0004672029,0.00023300563,0.00049624214,0.00033268513,0.0026025241],"category_scores_gemma":[0.0001845196,0.0001239193,0.00014126296,0.0004513455,0.00041343493,0.0002315941,0.00038330417,0.00048258677,0.00032927762],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022339178,0.0000887678,0.018581834,0.00010163796,0.000016757771,0.00029076793,0.00014005428,0.00037474962,0.9541415,0.0023460393,0.00030196496,0.023392556],"study_design_scores_gemma":[0.00017627845,0.00087167806,0.562194,0.000052482854,0.00008129928,0.0033240374,0.0007458652,0.0054550124,0.4081713,0.0050440393,0.013816957,0.00006705256],"about_ca_topic_score_codex":0.00054619525,"about_ca_topic_score_gemma":0.00079693424,"teacher_disagreement_score":0.0026025241,"about_ca_system_score_codex":0.00030019134,"about_ca_system_score_gemma":0.00021700372,"threshold_uncertainty_score":0.008706272},"labels":[],"label_agreement":null},{"id":"W2031080237","doi":"10.1088/0004-637x/778/2/135","title":"DOUBLE BLUE STRAGGLER SEQUENCES IN GLOBULAR CLUSTERS: THE CASE OF NGC 362","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Blue straggler; Physics; Astrophysics; Cluster (spacecraft); Population; Stars; Star cluster; Sequence (biology); Astronomy; Chemistry; Computer science; Medicine","score_opus":0.014430610973197776,"score_gpt":0.2378234373360677,"score_spread":0.22339282636286992,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031080237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988732,0.00008938798,0.00035357912,0.00002103442,0.0000017997381,0.0000036159481,0.00007455409,0.000022137592,0.0005607684],"genre_scores_gemma":[0.99914384,0.000028001066,0.0005109832,0.0000037000925,0.000003541839,0.0000015527119,0.000117300115,0.000007192448,0.00018381025],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976486,0.000031951015,0.000009462815,0.000083369356,0.00005058556,0.00005992364],"domain_scores_gemma":[0.99948823,0.00009482702,0.00011508569,0.00010599319,0.00004694712,0.00014885428],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035713013,0.00036906308,0.00022842347,0.0017097603,0.00073314866,0.0006557241,0.00031000166,0.00048364155,0.0006547871],"category_scores_gemma":[0.0011655932,0.00018099134,0.00023940479,0.001364679,0.0007652606,0.00028924854,0.00060372864,0.00018289547,0.00014908222],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067966926,0.000063880296,0.9085207,0.00006695254,0.00011336932,0.011026846,0.0020137043,0.014390258,0.043223344,0.0042344504,0.0009187798,0.014748024],"study_design_scores_gemma":[0.000025192689,0.00005844045,0.9674252,0.000013834173,0.00005478022,0.004207311,0.00075929204,0.018376006,0.0038906813,0.0023229185,0.0028123083,0.00005396746],"about_ca_topic_score_codex":0.029793119,"about_ca_topic_score_gemma":0.031741053,"teacher_disagreement_score":0.029793119,"about_ca_system_score_codex":0.0006362555,"about_ca_system_score_gemma":0.00031762867,"threshold_uncertainty_score":0.059239388},"labels":[],"label_agreement":null},{"id":"W2031100581","doi":"10.1088/0004-637x/766/1/21","title":"MULTI-WAVELENGTH STUDY OF A COMPLETE IRAC 3.6 μm SELECTED GALAXY SAMPLE: A FAIR CENSUS OF RED AND BLUE POPULATIONS AT REDSHIFTS 0.4-1.2","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Redshift; Galaxy; Stellar mass; Star formation; Astronomy; Luminous infrared galaxy; Luminosity; Galaxy formation and evolution","score_opus":0.025357239391037303,"score_gpt":0.2412870723148284,"score_spread":0.2159298329237911,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031100581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977082,0.00008044219,0.00069841207,0.000024190074,0.0000011985323,0.000007704423,0.0010259113,0.000019522264,0.00043435965],"genre_scores_gemma":[0.994406,0.00006584767,0.001466099,0.00003740669,0.00001077993,0.000020925318,0.0034002028,0.000021532253,0.0005712182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99964285,0.000054368913,0.000017479468,0.00012060269,0.000094764924,0.00006985822],"domain_scores_gemma":[0.99871135,0.000214337,0.00028415112,0.00026223954,0.00021593423,0.0003119876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005466062,0.00018963513,0.00027252748,0.0017942257,0.0003669602,0.00041775955,0.00040755642,0.00027970943,0.0010684269],"category_scores_gemma":[0.0010480798,0.00015864575,0.00034023094,0.0012186964,0.00019016891,0.0003631512,0.00073194026,0.00029482975,0.00056312437],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017999792,0.00016314597,0.9563714,0.000023980756,0.00013106772,0.00027447793,0.0005272065,0.0014582948,0.020894019,0.00041845546,0.0010012435,0.018556722],"study_design_scores_gemma":[0.0000027326118,0.000022023203,0.9977514,0.0000013275979,0.0000070678825,0.00013321028,0.00006854933,0.0010021494,0.0005010806,0.00004361052,0.00046363118,0.0000032889527],"about_ca_topic_score_codex":0.006333329,"about_ca_topic_score_gemma":0.012235879,"teacher_disagreement_score":0.006333329,"about_ca_system_score_codex":0.00023348688,"about_ca_system_score_gemma":0.00014910041,"threshold_uncertainty_score":0.012592912},"labels":[],"label_agreement":null},{"id":"W2031179207","doi":"10.1088/0004-637x/770/2/145","title":"VLBI ASTROMETRY OF PSR J2222-0137: A PULSAR DISTANCE MEASURED TO 0.4% ACCURACY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Physics; Astrometry; Pulsar; Very-long-baseline interferometry; Proper motion; Parallax; Astrophysics; Astronomy; Very Long Baseline Array; Radial velocity; Neutron star; Millisecond pulsar; Quasar; Stars; Galaxy","score_opus":0.013752252876357045,"score_gpt":0.3120368577941085,"score_spread":0.29828460491775144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031179207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96928674,0.00041021808,0.008352053,0.00018211322,0.000039080634,0.00008510115,0.00602084,0.0010313658,0.014592446],"genre_scores_gemma":[0.97990865,0.00012763022,0.013003722,0.000086255386,0.000022410988,0.000070979484,0.0047457186,0.00010080757,0.0019337616],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954283,0.000047257847,0.000035788562,0.00012777641,0.00017050841,0.000075869524],"domain_scores_gemma":[0.9994684,0.000028253791,0.00008527708,0.00015236916,0.00017498573,0.00009067265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005153573,0.00036718187,0.00040311247,0.0016376597,0.00047739924,0.0007017409,0.00062259944,0.00043784705,0.0016894902],"category_scores_gemma":[0.0013281576,0.00025183448,0.00017017734,0.0013743096,0.00021798753,0.00044326324,0.00058931997,0.00040643068,0.0018020674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047230907,0.00024209151,0.52415824,0.00017526207,0.00023606436,0.00040603292,0.001135844,0.0062181605,0.34702182,0.0031461862,0.010775879,0.10601211],"study_design_scores_gemma":[0.000046036308,0.00011186455,0.9275606,0.000034549976,0.00009084945,0.00039093412,0.00021776323,0.01952113,0.031243991,0.00032104552,0.020422082,0.00003913054],"about_ca_topic_score_codex":0.04099394,"about_ca_topic_score_gemma":0.055503037,"teacher_disagreement_score":0.04099394,"about_ca_system_score_codex":0.0010931841,"about_ca_system_score_gemma":0.0009487709,"threshold_uncertainty_score":0.08151066},"labels":[],"label_agreement":null},{"id":"W2031183485","doi":"10.1086/321417","title":"A Pair of Compact Red Galaxies at Redshift 2.38, Immersed in a 100 Kiloparsec Scale Lyα Nebula","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Astronomy; Elliptical galaxy; Peculiar galaxy; Galaxy; Disc; Luminous infrared galaxy; Lenticular galaxy","score_opus":0.010935537168573138,"score_gpt":0.22361962594965518,"score_spread":0.21268408878108203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031183485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996393,0.000102196114,0.000351515,0.0000975644,0.0000149598745,0.000029740937,0.00038923975,0.000050629023,0.0025712457],"genre_scores_gemma":[0.9932647,0.000054619573,0.0024945296,0.00006865801,0.000024650193,0.000020741298,0.001068248,0.0000075917765,0.0029964128],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982554,0.00001125311,0.000006200894,0.00006403044,0.00004475988,0.00004820116],"domain_scores_gemma":[0.99973255,0.000016217904,0.0000784449,0.000032423395,0.000014841226,0.00012542993],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017551398,0.00038502106,0.00044015332,0.0011710866,0.001087804,0.0005283875,0.0004251044,0.0007094733,0.0021929],"category_scores_gemma":[0.00035734757,0.00027976598,0.00023393589,0.00069533417,0.00041426517,0.00046743162,0.00075334165,0.00040665743,0.00060378393],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024634553,0.0015256978,0.71874833,0.0002116499,0.00020287622,0.01461146,0.0067019784,0.001135799,0.18386099,0.006146152,0.007341534,0.057050135],"study_design_scores_gemma":[0.00010985707,0.0010157634,0.95273167,0.000018798739,0.000070804635,0.013027432,0.0013947248,0.0019054158,0.0099173235,0.0015160674,0.018244864,0.00004727206],"about_ca_topic_score_codex":0.0027147455,"about_ca_topic_score_gemma":0.0044193347,"teacher_disagreement_score":0.0027147455,"about_ca_system_score_codex":0.0003638852,"about_ca_system_score_gemma":0.00017065818,"threshold_uncertainty_score":0.0073360205},"labels":[],"label_agreement":null},{"id":"W2031245901","doi":"10.1088/0004-637x/789/2/134","title":"THE INSIDE-OUT GROWTH OF THE MOST MASSIVE GALAXIES AT 0.3 &lt;<i>z</i>&lt; 0.9","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Surface brightness; Astrophysics; Galaxy; Physics; Effective radius; Sky; RADIUS; Cluster (spacecraft); Brightness; Galaxy cluster; Astronomy","score_opus":0.0053923079957716715,"score_gpt":0.19210536624206373,"score_spread":0.18671305824629206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031245901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9577649,0.0006405075,0.000466944,0.0015065189,0.000058331636,0.000009573606,0.005511942,0.0004457859,0.033595502],"genre_scores_gemma":[0.98974633,0.0001674261,0.0003034547,0.00010025701,0.000049575854,0.000006864639,0.0021775726,0.000067046894,0.007381527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989855,0.0000061434243,0.0000023042764,0.000024981347,0.000024354995,0.000043770477],"domain_scores_gemma":[0.99872345,0.00011907232,0.00027047712,0.00006384505,0.00029511465,0.0005279785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017337759,0.00013912082,0.00012831138,0.0022798446,0.00072265114,0.0017449254,0.00023861132,0.00044301173,0.00954233],"category_scores_gemma":[0.0012418955,0.00014710374,0.00018655829,0.0011885716,0.00034610112,0.0009958067,0.0008429098,0.0005381723,0.0018869315],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003241746,0.00009898898,0.865064,0.000069714704,0.000037048267,0.00040069062,0.005714987,0.00037816918,0.016763141,0.009227189,0.032947112,0.06897476],"study_design_scores_gemma":[0.0000026627117,0.000009927813,0.9878841,0.000008862442,0.000005092497,0.000070233946,0.0007964068,0.00024412593,0.0005920301,0.00045183417,0.009929135,0.000005556139],"about_ca_topic_score_codex":0.025935613,"about_ca_topic_score_gemma":0.04003168,"teacher_disagreement_score":0.025935613,"about_ca_system_score_codex":0.00058828766,"about_ca_system_score_gemma":0.0004195481,"threshold_uncertainty_score":0.051569343},"labels":[],"label_agreement":null},{"id":"W2031246503","doi":"10.1086/368356","title":"<i>XMM‐Newton</i>Observations of PSR B1823−13: An Asymmetric Synchrotron Nebula around a Vela‐like Pulsar","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Vela; Astrophysics; Pulsar wind nebula; Nebula; Supernova remnant; Astronomy; Supernova; Luminosity; RADIUS; Galaxy; Stars","score_opus":0.02190555009845243,"score_gpt":0.3111315914331764,"score_spread":0.289226041334724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031246503","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979418,0.00015299107,0.00023236008,0.00006460368,0.000004365373,0.000011804653,0.0005274222,0.0000743062,0.0009902209],"genre_scores_gemma":[0.99566525,0.00016559173,0.0017632779,0.00010035852,0.000032369797,0.00003368116,0.0015770185,0.000025575451,0.00063694734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999565,0.000003001092,0.0000025084319,0.000011607215,0.000013433001,0.000012962449],"domain_scores_gemma":[0.99984825,0.00000780491,0.00006214388,0.000007107867,0.000012666625,0.0000620998],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011886501,0.00028887155,0.00025746875,0.00083880866,0.00047889326,0.00041058447,0.00032191526,0.0003759047,0.0010405227],"category_scores_gemma":[0.00016037202,0.00013637844,0.00016684357,0.0004415239,0.00018970294,0.00016047084,0.00031086974,0.00034470955,0.0004065101],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081894576,0.00033981667,0.5654338,0.00016020506,0.00020345763,0.004055328,0.00073896523,0.00081901834,0.39819756,0.00038510736,0.003541829,0.025305904],"study_design_scores_gemma":[0.000043032192,0.00013632448,0.98989874,0.000015612242,0.000032421867,0.0015552163,0.000082961276,0.0005448083,0.00441218,0.00007993868,0.0031875381,0.000011244851],"about_ca_topic_score_codex":0.0029849953,"about_ca_topic_score_gemma":0.0068614217,"teacher_disagreement_score":0.0029849953,"about_ca_system_score_codex":0.00027382764,"about_ca_system_score_gemma":0.00011750087,"threshold_uncertainty_score":0.0059352517},"labels":[],"label_agreement":null},{"id":"W2031328795","doi":"10.1086/378265","title":"SN 1993J VLBI. III. The Evolution of the Radio Shell","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Nebula; Brightness; RADIUS; Shell (structure); Pulsar; Very-long-baseline interferometry; Ridge; Supernova; Core (optical fiber)","score_opus":0.006876613485355207,"score_gpt":0.20391431531538493,"score_spread":0.19703770183002972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031328795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97398937,0.00080614083,0.0020909393,0.00015364602,0.00004522426,0.000076274075,0.0106970705,0.00034477902,0.0117965825],"genre_scores_gemma":[0.9405083,0.00034092407,0.006778682,0.00021746971,0.000029709972,0.00009292991,0.045156278,0.00014226665,0.0067334133],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998807,0.000005106166,0.000005473156,0.00002816376,0.00004099355,0.000039555827],"domain_scores_gemma":[0.99983954,0.0000076389115,0.00004805487,0.000019015632,0.00005294734,0.00003277564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013992918,0.00034253942,0.00022556554,0.00095353986,0.0004020101,0.000556338,0.00030471582,0.00040219183,0.002823539],"category_scores_gemma":[0.0003525574,0.00024007111,0.0003016016,0.0007083667,0.00008070778,0.00016533243,0.00029833254,0.00030581915,0.001747503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021788445,0.00028228655,0.668116,0.00025377702,0.00050361356,0.0015059991,0.0003100601,0.0027022704,0.20939156,0.0013374218,0.016499221,0.09691898],"study_design_scores_gemma":[0.000025290185,0.000043530228,0.9802172,0.000012022837,0.00003765108,0.0010758245,0.000050448205,0.0023172426,0.006468711,0.00014678724,0.009594102,0.000011141459],"about_ca_topic_score_codex":0.026592694,"about_ca_topic_score_gemma":0.06253767,"teacher_disagreement_score":0.026592694,"about_ca_system_score_codex":0.0009192983,"about_ca_system_score_gemma":0.00018555736,"threshold_uncertainty_score":0.052875817},"labels":[],"label_agreement":null},{"id":"W2031332890","doi":"10.1086/308306","title":"The<i>Hubble Space Telescope</i>Key Project on the Extragalactic Distance Scale. XXV. A Recalibration of Cepheid Distances to Type Ia Supernovae and the Value of the Hubble Constant","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":160,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Hubble's law; Physics; Astrophysics; Galaxy; Cosmic distance ladder; Supernova; Astronomy; Metallicity; Redshift; Stars","score_opus":0.008202187389074736,"score_gpt":0.2296502432535397,"score_spread":0.22144805586446495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031332890","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.030012691,0.011040243,0.01677294,0.0071007195,0.0044294703,0.0007147532,0.71233714,0.0047218674,0.21287021],"genre_scores_gemma":[0.079319835,0.0060549383,0.042929787,0.0012301271,0.00078521355,0.0010693492,0.7743683,0.0007260138,0.09351637],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99930155,0.00008307055,0.000032764376,0.0001187576,0.0003700306,0.00009384712],"domain_scores_gemma":[0.99828905,0.000085201966,0.00045144308,0.00030241744,0.0005760759,0.00029587856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014895848,0.0009535767,0.0003848853,0.0028054442,0.0005723275,0.0015628351,0.0008288986,0.0004475415,0.0220948],"category_scores_gemma":[0.0016901401,0.00026269027,0.00034569256,0.0031443122,0.0002520586,0.0012356967,0.0019174161,0.0014401309,0.014225099],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014647092,0.000062153325,0.01719113,0.0002482913,0.00005057282,0.000046265224,0.000159266,0.00015135319,0.002016942,0.022659298,0.80362165,0.15364657],"study_design_scores_gemma":[0.00003961384,0.000042873475,0.14645047,0.00008240493,0.000013308527,0.000057972804,0.00006816419,0.00027169843,0.0007571979,0.0049158554,0.8472823,0.000018130157],"about_ca_topic_score_codex":0.029215038,"about_ca_topic_score_gemma":0.022529222,"teacher_disagreement_score":0.029215038,"about_ca_system_score_codex":0.0014852895,"about_ca_system_score_gemma":0.0017258453,"threshold_uncertainty_score":0.07391441},"labels":[],"label_agreement":null},{"id":"W2031520755","doi":"10.1088/0004-637x/751/1/24","title":"SPINDOWN OF ISOLATED NEUTRON STARS: GRAVITATIONAL WAVES OR MAGNETIC BRAKING?","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Neutron star; Gravitational wave; Neutron; Context (archaeology); Spin (aerodynamics); Saturation (graph theory); Magnetic damping; Magnetic field","score_opus":0.014617909831976646,"score_gpt":0.31314616922088306,"score_spread":0.2985282593889064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031520755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962838,0.00010218278,0.0028929126,0.000035146175,0.0000071465297,0.0000054662764,0.000027003434,0.00002372258,0.0006227194],"genre_scores_gemma":[0.9988952,0.000053538282,0.0007657187,0.000011269852,0.0000075429857,0.0000025013621,0.00004643805,0.000009212996,0.00020857014],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999541,0.0000072966677,0.0000026799637,0.000013483141,0.000009258939,0.000013167651],"domain_scores_gemma":[0.99937016,0.00017317303,0.0002237954,0.000059636932,0.000059267204,0.000114015114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000248725,0.0002988703,0.00039883802,0.00025366156,0.00025116932,0.00041788287,0.00035797566,0.00030795232,0.0006715847],"category_scores_gemma":[0.0013624285,0.00013345157,0.00022439093,0.00020479258,0.0004362516,0.00048469703,0.00039087315,0.00033599752,0.00012934918],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022167002,0.00053172704,0.36524427,0.00049824244,0.0003650911,0.005129191,0.001144175,0.130682,0.39233226,0.03154326,0.00097631733,0.069336824],"study_design_scores_gemma":[0.00016712522,0.0011275329,0.16005746,0.00004951145,0.00009766083,0.0013566397,0.00046971126,0.7524949,0.059407488,0.022290187,0.0023970278,0.000084779225],"about_ca_topic_score_codex":0.0008478421,"about_ca_topic_score_gemma":0.0011683862,"teacher_disagreement_score":0.0008478421,"about_ca_system_score_codex":0.00017527968,"about_ca_system_score_gemma":0.00011111862,"threshold_uncertainty_score":0.0022467375},"labels":[],"label_agreement":null},{"id":"W2031733552","doi":"10.1086/524978","title":"Light Propagation in Inhomogeneous Universes. V. Gravitational Lensing of Distant Supernovae","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Redshift; Supernova; Strong gravitational lensing; Universe; Weak gravitational lensing; Gravitational lensing formalism; Cosmology; Gravitational lens; Population; Shape of the universe; Astronomy; Galaxy","score_opus":0.009452622816173808,"score_gpt":0.22238933628324534,"score_spread":0.21293671346707152,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031733552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7090254,0.005652301,0.25145516,0.0006843466,0.000072837305,0.00005244433,0.00028562982,0.0005366892,0.03223526],"genre_scores_gemma":[0.9796514,0.0015776323,0.014359924,0.000058451747,0.000053955813,0.000017607046,0.00007750033,0.00002399951,0.004179526],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997876,0.00007065579,0.000008955213,0.0000339158,0.00006306897,0.000035826662],"domain_scores_gemma":[0.99753964,0.0012142417,0.0006587975,0.000295079,0.00016282016,0.00012950228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005164426,0.0004115198,0.00025940395,0.0015866372,0.0004890155,0.0007950046,0.00040953193,0.00037120088,0.0017872425],"category_scores_gemma":[0.003387566,0.00026793763,0.00033271592,0.0010627973,0.0013136012,0.0011845158,0.00066698604,0.0005247999,0.00023706547],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003440262,0.00007518649,0.050369967,0.00026708015,0.00019571221,0.0009044878,0.0008071505,0.10660922,0.06336791,0.7089634,0.0016645893,0.066431224],"study_design_scores_gemma":[0.00008807791,0.00018629385,0.06269557,0.000066843,0.00010723247,0.0011649259,0.00027699367,0.20701931,0.022703117,0.695641,0.009948378,0.00010231305],"about_ca_topic_score_codex":0.0039861547,"about_ca_topic_score_gemma":0.0025562225,"teacher_disagreement_score":0.0039861547,"about_ca_system_score_codex":0.0009457489,"about_ca_system_score_gemma":0.00019464993,"threshold_uncertainty_score":0.007925868},"labels":[],"label_agreement":null},{"id":"W2031857825","doi":"10.1088/0004-637x/715/1/589","title":"A NOVEL TECHNIQUE TO OBSERVE RAPIDLY PULSATING OBJECTS USING SPECTRAL WAVE-INTERACTION EFFECTS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Optics; Telescope; Interferometry; Detector; Wavefront; Cherenkov radiation; Measure (data warehouse); Noise (video); Astronomical interferometer; Beat (acoustics); Computer science","score_opus":0.01774361479942578,"score_gpt":0.25742045773615707,"score_spread":0.2396768429367313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031857825","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.083654106,0.0015505421,0.8994795,0.00057943555,0.00035941106,0.00018078306,0.00034663867,0.0021736058,0.011675917],"genre_scores_gemma":[0.33233425,0.0010839679,0.65822554,0.000500852,0.0003323803,0.00023837537,0.0002987292,0.0001574353,0.006828397],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99970883,0.000032938227,0.000011402097,0.00009505704,0.00012490412,0.000026851398],"domain_scores_gemma":[0.9995474,0.00009015889,0.00009016379,0.00014153015,0.00008384424,0.000046807105],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030039775,0.00033847874,0.00031576937,0.0013376927,0.0004956075,0.00054457673,0.000885291,0.0005783913,0.001719527],"category_scores_gemma":[0.00047267732,0.00029029118,0.00041155823,0.001004389,0.00063102477,0.0013769107,0.0010344125,0.0009832142,0.0007998694],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000165739,0.00015029093,0.0046745953,0.00018936979,0.00005915803,0.0002906313,0.00019148437,0.0009380508,0.78461635,0.015837664,0.0025794676,0.1903072],"study_design_scores_gemma":[0.00014662881,0.0017702174,0.030814976,0.00007227734,0.00024106145,0.010279061,0.000217068,0.08552649,0.7660228,0.018528908,0.08606307,0.00031738434],"about_ca_topic_score_codex":0.0002756536,"about_ca_topic_score_gemma":0.00068136625,"teacher_disagreement_score":0.001719527,"about_ca_system_score_codex":0.0002741019,"about_ca_system_score_gemma":0.0002879699,"threshold_uncertainty_score":0.0057524443},"labels":[],"label_agreement":null},{"id":"W2031956233","doi":"10.1086/308304","title":"The<i>Hubble Space Telescope</i>Key Project on the Extragalactic Distance Scale. XXVIII. Combining the Constraints on the Hubble Constant","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":539,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Hubble's law; Galaxy; Fundamental plane (elliptical galaxies); Milky Way; Surface brightness; Virgo Cluster; Local Group; Cosmic distance ladder","score_opus":0.010482223888047182,"score_gpt":0.2190869969992848,"score_spread":0.20860477311123762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2031956233","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.029885769,0.10493691,0.063158564,0.03537858,0.016975584,0.0008542168,0.1313345,0.004136835,0.61333907],"genre_scores_gemma":[0.19917871,0.07024635,0.11944849,0.0035265516,0.0057560923,0.0012468752,0.21982262,0.0014194307,0.37935492],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9995788,0.0000586354,0.000014019155,0.00006588237,0.00021420751,0.000068388734],"domain_scores_gemma":[0.99904686,0.000085550426,0.00021748594,0.00015845709,0.00026945258,0.00022230105],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014304584,0.0013688001,0.0004999278,0.0026398608,0.0004887364,0.0018998446,0.0009007916,0.00070123014,0.01870425],"category_scores_gemma":[0.0015439346,0.0003075483,0.00043850264,0.0027651805,0.00057214644,0.0014500446,0.0016510119,0.0015294702,0.010302999],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019648127,0.000080129044,0.007338795,0.00036337532,0.000067596244,0.00010393011,0.000108476226,0.0015795055,0.0023529583,0.08909318,0.612944,0.28577155],"study_design_scores_gemma":[0.00004263317,0.00005519321,0.040941887,0.00019035202,0.000013336074,0.000088774774,0.000057734793,0.0013166394,0.00082275254,0.031102119,0.9253444,0.000024271501],"about_ca_topic_score_codex":0.015267672,"about_ca_topic_score_gemma":0.010063028,"teacher_disagreement_score":0.01870425,"about_ca_system_score_codex":0.0025103074,"about_ca_system_score_gemma":0.0017370393,"threshold_uncertainty_score":0.062572},"labels":[],"label_agreement":null},{"id":"W2032082898","doi":"10.1086/589610","title":"Time‐Resolved<i>FUSE</i>Spectroscopy of the LMC WC + O Binaries Br 22 and Br 32","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Emission spectrum; Spectral line; Absorption spectroscopy; Absorption (acoustics); Spectroscopy; Astronomy; Optics","score_opus":0.008700548033376623,"score_gpt":0.20914755184780398,"score_spread":0.20044700381442737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032082898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99850804,0.000078459634,0.00013753897,0.000014440124,0.0000030521835,0.0000034514105,0.00030214098,0.0000343836,0.0009184411],"genre_scores_gemma":[0.99856275,0.000027035509,0.00032299384,0.000020480176,0.0000037907573,0.000005048242,0.000833818,0.000011231803,0.00021285911],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989486,0.0000047252965,0.0000039012466,0.00004014752,0.000025305271,0.00003106706],"domain_scores_gemma":[0.9998301,0.000009467097,0.00006383855,0.000020564923,0.000019834586,0.00005613803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014289845,0.00037098755,0.00023673433,0.0007804311,0.00047653267,0.00040575687,0.0003992057,0.0004037237,0.0006704847],"category_scores_gemma":[0.00026043958,0.00021641236,0.00014431008,0.0005916207,0.00015327362,0.0002616539,0.0004215719,0.00040179596,0.000233811],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013420025,0.0002811291,0.38691837,0.00007274864,0.0002205522,0.0012300182,0.00064920034,0.003341998,0.5862977,0.0006201325,0.001521768,0.017504426],"study_design_scores_gemma":[0.000023132025,0.000109511806,0.98649186,0.000006593199,0.000036588404,0.00022277667,0.000132658,0.0040035928,0.007694295,0.00008842854,0.0011728808,0.000017587314],"about_ca_topic_score_codex":0.010635975,"about_ca_topic_score_gemma":0.017901435,"teacher_disagreement_score":0.010635975,"about_ca_system_score_codex":0.00053228915,"about_ca_system_score_gemma":0.00012312553,"threshold_uncertainty_score":0.021148145},"labels":[],"label_agreement":null},{"id":"W2032113670","doi":"10.1086/517922","title":"AEGIS: Host Galaxy Morphologies of X-Ray-selected and Infrared-selected Active Galactic Nuclei at 0.2 ≤ <i>z</i> &lt; 1.2","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Redshift; Population; Infrared; Galaxy formation and evolution; Flux (metallurgy); Astronomy; Chemistry","score_opus":0.006149231179827002,"score_gpt":0.20702341087430848,"score_spread":0.2008741796944815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032113670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925991,0.00011698083,0.00021640817,0.000018141158,0.0000044713806,0.000009315746,0.0029607345,0.00006773818,0.004007054],"genre_scores_gemma":[0.9943467,0.00008237638,0.00058989733,0.000016842634,0.000005010798,0.0000049745872,0.003915638,0.000025797324,0.0010127637],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999596,0.000003055064,0.0000033044844,0.0000139476815,0.000009405398,0.000010639919],"domain_scores_gemma":[0.9998325,0.000013830865,0.00006769838,0.00001878321,0.00002386336,0.000043327287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009520724,0.0001830305,0.00012475051,0.00107494,0.00015041888,0.000400146,0.00013688655,0.00011009923,0.0026429195],"category_scores_gemma":[0.0002328173,0.000090838854,0.00013463231,0.0004062703,0.00011679075,0.00029643238,0.0003295788,0.00011105613,0.00056692975],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044464073,0.00003352119,0.92281955,0.00004956011,0.00010797868,0.00023078397,0.00027262818,0.00073715975,0.057040907,0.0005303545,0.001935533,0.015797406],"study_design_scores_gemma":[0.000005336422,0.000015044185,0.99649847,0.0000027914214,0.000011821759,0.00018455571,0.000082034305,0.00053840835,0.0017636288,0.00004510646,0.0008505447,0.0000021834046],"about_ca_topic_score_codex":0.009809187,"about_ca_topic_score_gemma":0.019706113,"teacher_disagreement_score":0.009809187,"about_ca_system_score_codex":0.00031949038,"about_ca_system_score_gemma":0.00006143399,"threshold_uncertainty_score":0.01950419},"labels":[],"label_agreement":null},{"id":"W2032125763","doi":"10.1086/318682","title":"Molecular Gas and the Modest Star Formation Efficiency in the “Antennae” Galaxies: Arp 244 = NGC 4038/9","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; University of Toronto","funders":"","keywords":"Star formation; Molecular cloud; Stars; Flux (metallurgy); H II region; Stellar mass; Interstellar medium","score_opus":0.010049957621788471,"score_gpt":0.22355902851427326,"score_spread":0.21350907089248478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032125763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99759656,0.00017057384,0.000053371114,0.000040248917,0.0000030032377,0.0000010867333,0.00020726699,0.000013400545,0.0019144774],"genre_scores_gemma":[0.99935883,0.000065211534,0.00005300229,0.000009848107,0.000015653275,0.0000014234871,0.00020664501,0.0000037674884,0.0002856298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989474,0.000014956888,0.0000074006666,0.000040363728,0.000016489019,0.000026094855],"domain_scores_gemma":[0.9997017,0.000039991355,0.00014196066,0.000026089716,0.000019003111,0.00007130087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012685928,0.00023049705,0.00015450033,0.0009633839,0.00032926505,0.0006937426,0.00015698835,0.00021365192,0.0030815923],"category_scores_gemma":[0.0003758662,0.00009056692,0.00008568746,0.00048719143,0.00037307187,0.00026256507,0.0003311034,0.00019737764,0.00063653634],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029156814,0.00007985646,0.96474785,0.000023610297,0.000045157944,0.00092384074,0.00034398775,0.00019422756,0.022777406,0.0007658179,0.00089334324,0.008913374],"study_design_scores_gemma":[0.000003034531,0.000028722596,0.99771786,0.000002345217,0.0000076719425,0.0007572999,0.00010811341,0.000060701674,0.00048370403,0.00010953553,0.00071888923,0.0000021625435],"about_ca_topic_score_codex":0.0017402406,"about_ca_topic_score_gemma":0.001501677,"teacher_disagreement_score":0.0030815923,"about_ca_system_score_codex":0.00015993648,"about_ca_system_score_gemma":0.00005154888,"threshold_uncertainty_score":0.010308921},"labels":[],"label_agreement":null},{"id":"W2032126520","doi":"10.1086/528796","title":"Timing the Nearby Isolated Neutron Star RX J1856.5-3754","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Neutron star; Physics; Astrophysics; Stars; Black-body radiation; Magnetic field; Field (mathematics); Radiation; Nuclear physics","score_opus":0.021921318223033837,"score_gpt":0.23182118829203785,"score_spread":0.209899870069004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032126520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972938,0.00015060967,0.0005643709,0.000027795526,0.000009638719,0.0000043165974,0.00020036669,0.000030716008,0.0017184761],"genre_scores_gemma":[0.99858826,0.00003024309,0.00051656313,0.000007120729,0.0000061553824,0.0000016829645,0.000305737,0.0000072191374,0.00053688174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999094,0.000011408506,0.000005483459,0.00003560132,0.000022792252,0.000015317706],"domain_scores_gemma":[0.99984765,0.000015116011,0.00006141996,0.000019574165,0.000021259231,0.000034996672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016279539,0.00018711554,0.000212751,0.0003242639,0.000285226,0.00029878796,0.00026040286,0.00018315496,0.0011775352],"category_scores_gemma":[0.00046095552,0.00009778951,0.00016538874,0.00019954772,0.00020862493,0.00013699377,0.00036388432,0.00016356932,0.0002624194],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008527563,0.00013771115,0.81863415,0.00020041133,0.00021659961,0.0016647587,0.000598683,0.0072905524,0.13034785,0.0035200855,0.0015124055,0.035024032],"study_design_scores_gemma":[0.00002977122,0.00021367069,0.97857225,0.000014630539,0.000066651904,0.0005289298,0.000120067416,0.008214925,0.007955021,0.0004979025,0.0037722944,0.00001398809],"about_ca_topic_score_codex":0.003034879,"about_ca_topic_score_gemma":0.0057540946,"teacher_disagreement_score":0.003034879,"about_ca_system_score_codex":0.00035416632,"about_ca_system_score_gemma":0.00014135716,"threshold_uncertainty_score":0.006034434},"labels":[],"label_agreement":null},{"id":"W2032141873","doi":"10.1086/588551","title":"An Arc of Young Stars in the Halo of M82","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Astrophysics; Physics; Metallicity; Halo; Galaxy; Arc (geometry); Astronomy; Geometry","score_opus":0.014645521731825758,"score_gpt":0.23130210633092047,"score_spread":0.2166565845990947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032141873","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980596,0.00038745845,0.000040483574,0.000022705675,0.0000010073646,0.000001221702,0.00003386415,0.0000087322305,0.0014449499],"genre_scores_gemma":[0.9992269,0.00016258542,0.000083774685,0.000016561442,0.0000057429124,8.9969905e-7,0.00008124795,0.0000037101813,0.00041860988],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995553,0.0000048041998,0.0000025776608,0.000012463429,0.000012879273,0.000011736636],"domain_scores_gemma":[0.99978715,0.000019399784,0.00006627438,0.000020106398,0.00003934266,0.00006781847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011577055,0.0001034997,0.00012999128,0.00082717853,0.00051136175,0.00046488325,0.00011048205,0.00015356137,0.00088111026],"category_scores_gemma":[0.00029903476,0.00013343936,0.00009019658,0.00068561453,0.00024515597,0.0002715124,0.000566191,0.00009721668,0.00024107896],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002590282,0.000056689325,0.9154445,0.00007329766,0.000055253204,0.002098853,0.0026104758,0.00070348335,0.05661742,0.0014263327,0.000859427,0.019795354],"study_design_scores_gemma":[0.000005766567,0.000051130854,0.99566466,0.000006728113,0.000019451107,0.0006789398,0.00031890048,0.00023590976,0.0006466021,0.00020618708,0.0021612158,0.0000045213123],"about_ca_topic_score_codex":0.0035847654,"about_ca_topic_score_gemma":0.005955824,"teacher_disagreement_score":0.0035847654,"about_ca_system_score_codex":0.0003293812,"about_ca_system_score_gemma":0.0001241304,"threshold_uncertainty_score":0.0071278214},"labels":[],"label_agreement":null},{"id":"W2032168281","doi":"10.1088/0004-637x/747/1/4","title":"ON THE DYNAMICS AND TIDAL DISSIPATION RATE OF THE WHITE DWARF IN 4U 1820-30","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Libration (molecule); Eccentricity (behavior); Orbital period; Astrophysics; Orbit (dynamics); Lagrangian point; Binary number; Stars; Classical mechanics; Geometry; Mathematics; Point (geometry)","score_opus":0.010323442194830655,"score_gpt":0.2244261985418886,"score_spread":0.21410275634705794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032168281","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99935573,0.000028963166,0.00009106389,0.00001822847,9.643659e-7,0.0000010287132,0.000019159539,0.000006339475,0.00047853534],"genre_scores_gemma":[0.9995875,0.000016589045,0.0000886941,0.0000037322916,0.0000013087089,0.0000015911827,0.000048817146,0.000004805877,0.00024697214],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996495,0.0000045056963,0.000001858653,0.000011157066,0.000007074091,0.000010496499],"domain_scores_gemma":[0.99982697,0.000036265792,0.000065284716,0.000011579487,0.000017481152,0.000042387284],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012886019,0.00016724544,0.00028992412,0.00054284866,0.00047604597,0.0005326348,0.00022271005,0.00024272897,0.00071313104],"category_scores_gemma":[0.00064650824,0.00017901346,0.00014439116,0.0002837743,0.00040065747,0.00023250122,0.00035685615,0.0002191186,0.00024567216],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081915286,0.00017338482,0.73540497,0.00008954823,0.00010885538,0.0022867532,0.001401531,0.05089237,0.17873152,0.0075586378,0.00086022273,0.021673078],"study_design_scores_gemma":[0.00004388084,0.00022657984,0.87048876,0.000015269065,0.000031562322,0.0005114189,0.00048618793,0.11416912,0.0106207635,0.0017031714,0.0016404612,0.00006275062],"about_ca_topic_score_codex":0.0054433085,"about_ca_topic_score_gemma":0.004452821,"teacher_disagreement_score":0.0054433085,"about_ca_system_score_codex":0.0008020274,"about_ca_system_score_gemma":0.00021531021,"threshold_uncertainty_score":0.01082325},"labels":[],"label_agreement":null},{"id":"W2032204072","doi":"10.1088/0004-637x/725/2/2117","title":"PERPENDICULAR DIFFUSION OF COSMIC RAYS FOR A GOLDREICH-SRIDHAR SPECTRUM","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Cosmic ray; Diffusion; Perpendicular; Computational physics; Anisotropic diffusion; Shock (circulatory); Turbulence; Anisotropy; Astrophysics; Statistical physics; Mechanics; Optics; Geometry; Quantum mechanics","score_opus":0.004190148742694002,"score_gpt":0.21862437804558968,"score_spread":0.21443422930289568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032204072","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8364631,0.00068251725,0.14547771,0.0003526833,0.00007042817,0.00005711318,0.00023767063,0.00020421422,0.016454654],"genre_scores_gemma":[0.9844119,0.00045351696,0.010827167,0.00003404025,0.000018982551,0.000027515656,0.00015969531,0.000075151096,0.0039919484],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999056,0.000026021826,0.000007338617,0.000017648435,0.000025598905,0.000017731254],"domain_scores_gemma":[0.99961555,0.00012236334,0.000081693746,0.000037358455,0.000073656985,0.00006933993],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004356831,0.0007995402,0.00032684903,0.00091221684,0.00035296433,0.00095406966,0.00052188174,0.0006201252,0.0022808218],"category_scores_gemma":[0.001354421,0.00020825645,0.00083624927,0.0004303402,0.00064519496,0.0011098937,0.0005932836,0.0005575205,0.00045717083],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014893063,0.00006852811,0.007934817,0.00009605108,0.000048120874,0.0005053354,0.0001311715,0.7628239,0.017462367,0.20411815,0.0010693319,0.005593342],"study_design_scores_gemma":[0.000009419242,0.0000124174385,0.0007733301,0.0000044593944,0.000006456493,0.00006830536,0.000018155095,0.98791426,0.0006631605,0.010271833,0.00024337531,0.000014906937],"about_ca_topic_score_codex":0.0062541403,"about_ca_topic_score_gemma":0.003456546,"teacher_disagreement_score":0.0062541403,"about_ca_system_score_codex":0.0010744521,"about_ca_system_score_gemma":0.00056870625,"threshold_uncertainty_score":0.012435496},"labels":[],"label_agreement":null},{"id":"W2032255556","doi":"10.1088/0004-637x/730/2/80","title":"EVIDENCE FOR AN FU ORIONIS-LIKE OUTBURST FROM A CLASSICAL T TAURI STAR","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Jet Propulsion Laboratory; Space Telescope Science Institute; Harvard University; Smithsonian Astrophysical Observatory; U.S. Department of Energy; W. M. Keck Foundation; Office of Science; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; T Tauri star; Supergiant; Brightness; Nebula; Spectral line; Astronomy; Infrared; Photosphere; Stars","score_opus":0.08610087621111416,"score_gpt":0.2950660192873999,"score_spread":0.20896514307628572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032255556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993253,0.000047669564,0.000043970238,0.0000153742,0.0000045265024,0.000004405744,0.000059411846,0.000008275752,0.0004910686],"genre_scores_gemma":[0.9991586,0.000050554932,0.0001451697,0.000030246198,0.000017799011,0.0000046062555,0.0003013821,0.0000025400127,0.00028915578],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993646,0.0000032832202,0.0000046980695,0.000023236922,0.000013118098,0.00001926313],"domain_scores_gemma":[0.99947494,0.000041018633,0.00022886104,0.00003691929,0.000043397547,0.0001749168],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001362725,0.0002519327,0.0002394016,0.0004668013,0.00048861944,0.00038384355,0.00031661254,0.00043294628,0.0014817506],"category_scores_gemma":[0.000390034,0.00013948703,0.00015208044,0.00031014415,0.0003748419,0.00027015005,0.00046510578,0.00040132186,0.00032212186],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045612315,0.00013805571,0.91066015,0.00004702999,0.000022067625,0.0075054504,0.0007042853,0.0000757568,0.073312946,0.000107998945,0.000281776,0.0066882344],"study_design_scores_gemma":[0.000005054912,0.00014872717,0.99654454,0.000003080088,0.0000054122993,0.00204336,0.00011734292,0.000057801102,0.0006539737,0.000025839754,0.00039257604,0.0000022367121],"about_ca_topic_score_codex":0.00206374,"about_ca_topic_score_gemma":0.0047039585,"teacher_disagreement_score":0.00206374,"about_ca_system_score_codex":0.00026488485,"about_ca_system_score_gemma":0.00011034276,"threshold_uncertainty_score":0.004956901},"labels":[],"label_agreement":null},{"id":"W2032480060","doi":"10.1088/0004-637x/772/1/74","title":"DENSITY AND ECCENTRICITY OF<i>KEPLER</i>PLANETS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planet; Physics; Photoevaporation; Astrophysics; Eccentricity (behavior); Radial velocity; RADIUS; Astronomy; Stars; Jovian; Saturn; Protoplanetary disk","score_opus":0.00771033812484818,"score_gpt":0.1992189743581095,"score_spread":0.19150863623326134,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032480060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99923027,0.000037960763,0.00005382947,0.0000054055013,5.815748e-7,8.4591437e-7,0.00025069877,0.0000072713456,0.00041311473],"genre_scores_gemma":[0.99902666,0.000026241252,0.000082709965,0.0000020421012,0.0000024160893,0.000001925806,0.00069348165,0.000003454636,0.00016097665],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998568,0.0000143402085,0.000013074179,0.000061172315,0.00002749021,0.00002701414],"domain_scores_gemma":[0.99893576,0.0002029005,0.00057536166,0.00007735801,0.000104252256,0.00010441823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015239515,0.00011444801,0.00014724491,0.0015733473,0.0002440217,0.00038729463,0.00020952399,0.00021898933,0.0012004869],"category_scores_gemma":[0.0014884582,0.00014136484,0.000110541805,0.00096880866,0.00024882416,0.00041157295,0.00037391644,0.00013025421,0.00042124733],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010589888,0.00001102284,0.9879018,0.00001372939,0.000027106062,0.00013033277,0.00040698727,0.00051056163,0.006326919,0.00014087482,0.0002125816,0.00421224],"study_design_scores_gemma":[0.00000204125,0.000024796587,0.9973814,0.0000022125505,0.00000652995,0.00033394533,0.00011955364,0.0006542673,0.00094678265,0.00003630701,0.0004872007,0.0000048347424],"about_ca_topic_score_codex":0.001985132,"about_ca_topic_score_gemma":0.0015510102,"teacher_disagreement_score":0.001985132,"about_ca_system_score_codex":0.00023902186,"about_ca_system_score_gemma":0.00006431893,"threshold_uncertainty_score":0.0040160418},"labels":[],"label_agreement":null},{"id":"W2032521681","doi":"10.1088/0004-637x/757/2/122","title":"THE SUPPRESSION OF STAR FORMATION AND THE EFFECT OF THE GALAXY ENVIRONMENT IN LOW-REDSHIFT GALAXY GROUPS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Interacting galaxy; Lenticular galaxy; Galaxy; Star formation; Galaxy group; Dwarf galaxy; Galaxy merger; Galaxy formation and evolution; Protogalaxy","score_opus":0.003397894838871274,"score_gpt":0.18788724551202074,"score_spread":0.18448935067314948,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032521681","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99954236,0.000050485774,0.00016315996,0.000006899011,3.4396305e-7,8.6146434e-7,0.00002705736,0.0000072111097,0.00020173099],"genre_scores_gemma":[0.99975246,0.00001750142,0.00008797392,0.000005664457,0.0000013321877,0.0000010265838,0.000058678088,0.0000028660745,0.000072413495],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998292,0.000035031757,0.000010042184,0.00005054753,0.000033668253,0.000041562496],"domain_scores_gemma":[0.99896944,0.0001870527,0.00040690677,0.00018838212,0.000053102034,0.00019509127],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030452298,0.00019355264,0.00028796823,0.00050614553,0.00024426053,0.00056180556,0.00024020961,0.00022411808,0.0007735187],"category_scores_gemma":[0.0010643014,0.00014671263,0.00024762045,0.00031159757,0.0005295163,0.0003605165,0.00064136443,0.00020214467,0.00016534253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030213452,0.00004172835,0.8923836,0.00003302685,0.00010219095,0.00006799631,0.00037058064,0.0019918147,0.09661081,0.00030220728,0.0000673925,0.0077264523],"study_design_scores_gemma":[0.000002648085,0.00005795183,0.995227,0.0000012118916,0.000013847069,0.000043030424,0.000053788033,0.00081813417,0.0035297622,0.00014469173,0.0001053638,0.0000026174807],"about_ca_topic_score_codex":0.001828177,"about_ca_topic_score_gemma":0.0017734034,"teacher_disagreement_score":0.001828177,"about_ca_system_score_codex":0.00024993642,"about_ca_system_score_gemma":0.000095218675,"threshold_uncertainty_score":0.0036351085},"labels":[],"label_agreement":null},{"id":"W2032651825","doi":"10.1086/426897","title":"Intermittency and Phase Persistence in a Babcock-Leighton Model of the Solar Cycle","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Intermittency; Physics; Dynamo; Amplitude; Sunspot; Astrophysics; Solar cycle; Solar dynamo; Convection zone; Solar cycle 24; Solar minimum; Atmospheric sciences; Solar wind; Magnetic field; Meteorology; Dynamo theory; Stars; Turbulence; Optics","score_opus":0.010135218194903338,"score_gpt":0.22816052343290485,"score_spread":0.2180253052380015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032651825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9846677,0.00014625292,0.009927066,0.00029756624,0.000020864933,0.00001618757,0.00013137811,0.00006985521,0.0047230357],"genre_scores_gemma":[0.99787116,0.000077837394,0.001211647,0.000024215866,0.000008688172,0.00001800741,0.00006374544,0.000012906915,0.0007116624],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998977,0.000042921387,0.0000049951645,0.000015704207,0.000015132171,0.000023558938],"domain_scores_gemma":[0.9995994,0.00021225383,0.000056994075,0.000019430112,0.000032598113,0.00007936068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028121806,0.0002783354,0.0004844072,0.00036346877,0.00054814236,0.0008103545,0.0006859652,0.0008547686,0.0017978454],"category_scores_gemma":[0.0019191387,0.00026311187,0.00034308454,0.0004424388,0.0008413486,0.00075955695,0.0005876581,0.0005209424,0.0001111057],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008118782,0.000030851676,0.0041439645,0.0000105626195,0.000022288272,0.000115187635,0.00008015262,0.9848258,0.0006097269,0.008998121,0.00023997962,0.00084210053],"study_design_scores_gemma":[0.00002137637,0.000016601545,0.0004947998,0.0000017897601,0.0000046604137,0.000009224822,0.00001507899,0.9975074,0.000054852197,0.0017573038,0.00011299292,0.0000040599416],"about_ca_topic_score_codex":0.02549101,"about_ca_topic_score_gemma":0.010082113,"teacher_disagreement_score":0.02549101,"about_ca_system_score_codex":0.000850727,"about_ca_system_score_gemma":0.0006546751,"threshold_uncertainty_score":0.050685227},"labels":[],"label_agreement":null},{"id":"W2032676265","doi":"10.1088/0004-637x/751/1/66","title":"<i>HUBBLE SPACE TELESCOPE</i>FUV SPECTRA OF THE POST-COMMON-ENVELOPE HYADES BINARY V471 Tauri","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency","funders":"","keywords":"Physics; Astrophysics; T Tauri star; White dwarf; Astronomy; Accretion (finance); Spectral line; Zeeman effect; Rotation period; Stars; Magnetic field","score_opus":0.009087736113001366,"score_gpt":0.2188524220526419,"score_spread":0.20976468593964054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032676265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983986,0.000055060078,0.00007970181,0.000010611888,0.0000020719988,0.0000025986908,0.00073440507,0.000017486154,0.00069943647],"genre_scores_gemma":[0.99512523,0.0000664687,0.00043259768,0.000014710606,0.000010569292,0.000005882214,0.0035727196,0.000011715161,0.00076001283],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995005,0.00000435858,0.00000285122,0.000013701958,0.0000141447,0.000014860121],"domain_scores_gemma":[0.9997907,0.000025808036,0.0000696344,0.000025399537,0.00004237067,0.000046054156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012589294,0.0001710428,0.00013124938,0.0007989537,0.00032884342,0.00037191107,0.00017205057,0.00013908473,0.001551355],"category_scores_gemma":[0.00019495602,0.00008397698,0.00015716838,0.00046511882,0.00008887856,0.00010559559,0.00016175034,0.00015956999,0.00038543312],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008649166,0.0001853507,0.70789,0.00010497002,0.00015015183,0.00080516934,0.0009987374,0.0012579273,0.26502123,0.00025869455,0.0015589277,0.020903846],"study_design_scores_gemma":[0.0000037159691,0.00004146857,0.99456704,0.0000029350804,0.000012425525,0.000101591955,0.000045403976,0.00027538554,0.00434183,0.000013355099,0.00059232756,0.0000024681606],"about_ca_topic_score_codex":0.004872462,"about_ca_topic_score_gemma":0.007544584,"teacher_disagreement_score":0.004872462,"about_ca_system_score_codex":0.00024574055,"about_ca_system_score_gemma":0.00007353129,"threshold_uncertainty_score":0.009688199},"labels":[],"label_agreement":null},{"id":"W2032697794","doi":"10.1086/309364","title":"A New View of Cold H<scp>i</scp>Clouds in the Milky Way","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; University of Calgary","funders":"","keywords":"Physics; Milky Way; Astrophysics; Galactic plane; Population; Molecular cloud; Line (geometry); Astronomy; Galaxy; Stars; Geometry","score_opus":0.010657928113013984,"score_gpt":0.23482914879430394,"score_spread":0.22417122068128997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032697794","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9859483,0.0017231265,0.00220068,0.0006510548,0.000016873102,0.0000049109567,0.000295517,0.000078810655,0.009080686],"genre_scores_gemma":[0.99751055,0.00040142128,0.000971667,0.00014842817,0.00005712029,0.0000022640452,0.0002049743,0.000014439545,0.00068916654],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994934,0.0000024440565,0.00000174034,0.000013928053,0.000015663525,0.000016903423],"domain_scores_gemma":[0.9998429,0.000018542172,0.000055021854,0.000024213783,0.000017804934,0.00004153806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000089822184,0.00013089018,0.0002835447,0.0006809829,0.0004731897,0.0013931786,0.00045007592,0.0002894665,0.0012031886],"category_scores_gemma":[0.00026119704,0.00015042376,0.00018033174,0.0007917778,0.00086498604,0.0011562313,0.00059947645,0.0004852097,0.00012799415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003277568,0.000041288426,0.7727125,0.00033320917,0.00020890111,0.001512826,0.0030722576,0.0039840573,0.097740486,0.023490584,0.0044635013,0.09211256],"study_design_scores_gemma":[0.000014401693,0.0000486142,0.9699046,0.000034309003,0.000046984154,0.0007533494,0.00091508083,0.0020967855,0.0020679764,0.00830145,0.015796537,0.000019872232],"about_ca_topic_score_codex":0.011288075,"about_ca_topic_score_gemma":0.02607844,"teacher_disagreement_score":0.011288075,"about_ca_system_score_codex":0.00059958355,"about_ca_system_score_gemma":0.00032155853,"threshold_uncertainty_score":0.022444725},"labels":[],"label_agreement":null},{"id":"W2032752125","doi":"10.1086/427144","title":"The Phoenix Deep Survey: The Clustering and Environment of Extremely Red Objects","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Amplitude; Cluster analysis; Phoenix; Flux (metallurgy); Astronomy; Smoothing; Correlation function (quantum field theory); Statistics; Optics; Geography; Computer science; Artificial intelligence","score_opus":0.009563859577784283,"score_gpt":0.19845206481580738,"score_spread":0.1888882052380231,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032752125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926322,0.00014455884,0.0016605483,0.00008088742,0.000002755668,0.000024175906,0.0030779382,0.000038502563,0.0023384534],"genre_scores_gemma":[0.9862708,0.00035772735,0.005289084,0.00011423473,0.000026387814,0.000031193427,0.0058479756,0.000035029927,0.0020276203],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978894,0.000029141134,0.0000066086504,0.00008824291,0.000043345735,0.000043787262],"domain_scores_gemma":[0.99951804,0.00006733421,0.0001802084,0.00007551494,0.000047671754,0.0001113126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004318371,0.00024048163,0.00020205986,0.0011936198,0.00028868762,0.00063786353,0.00030587835,0.00017053976,0.0011916101],"category_scores_gemma":[0.000694156,0.00013399067,0.000097998796,0.0014498008,0.00022201295,0.0005526946,0.0011641047,0.00039829337,0.00025055723],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015601292,0.00005528931,0.9635027,0.00004303797,0.00007094388,0.00020256825,0.00061196653,0.0009505268,0.010353117,0.00058292015,0.0014793569,0.021991538],"study_design_scores_gemma":[0.00000338885,0.000014016658,0.9966852,0.0000034780855,0.000007649457,0.0000871484,0.00013398095,0.00043139711,0.00064538553,0.00006821685,0.0019163006,0.0000037182585],"about_ca_topic_score_codex":0.012740605,"about_ca_topic_score_gemma":0.020112801,"teacher_disagreement_score":0.012740605,"about_ca_system_score_codex":0.00032038408,"about_ca_system_score_gemma":0.00015654393,"threshold_uncertainty_score":0.025332928},"labels":[],"label_agreement":null},{"id":"W2032756593","doi":"10.1086/504520","title":"On the Primordial Scenario for Abundance Variations within Globular Clusters: The Isochrone Test","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Horizontal branch; Red-giant branch; Stars; Luminosity; Red giant; Stellar evolution; Abundance (ecology); Asymptotic giant branch","score_opus":0.009201899533108952,"score_gpt":0.21694966435552038,"score_spread":0.20774776482241142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032756593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90307754,0.00051436294,0.08087699,0.0011399572,0.00007604376,0.000056009,0.00029285168,0.0003438521,0.013622375],"genre_scores_gemma":[0.99272,0.00006566034,0.0064630974,0.00006885701,0.000029057017,0.000039348273,0.0001780077,0.0000676285,0.0003683006],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9980622,0.0010661865,0.000055097036,0.00049042585,0.00014586271,0.00018017825],"domain_scores_gemma":[0.966296,0.025931407,0.0020494666,0.0037437605,0.0009372527,0.0010421684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010643158,0.00050802575,0.00064748776,0.0007729012,0.0011548162,0.002535238,0.001933847,0.0017038252,0.004248789],"category_scores_gemma":[0.043437067,0.0003016217,0.0010179935,0.00072765676,0.0027722334,0.0032006586,0.0015514696,0.0012451373,0.00065017893],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002530338,0.00026304237,0.2784975,0.00016225858,0.00038135846,0.0013771055,0.0017362495,0.08200387,0.006175086,0.5844414,0.0016169631,0.040814847],"study_design_scores_gemma":[0.0004967367,0.00062875444,0.11540918,0.000087153196,0.0002975242,0.0010461902,0.0008561455,0.5876697,0.003315329,0.28643885,0.0035913382,0.00016305251],"about_ca_topic_score_codex":0.0017545744,"about_ca_topic_score_gemma":0.00086959737,"teacher_disagreement_score":0.010643158,"about_ca_system_score_codex":0.0007944294,"about_ca_system_score_gemma":0.000785047,"threshold_uncertainty_score":0.05628705},"labels":[],"label_agreement":null},{"id":"W2032840199","doi":"10.1088/0004-637x/773/1/79","title":"SHOCK EMERGENCE IN SUPERNOVAE: LIMITING CASES AND ACCURATE APPROXIMATIONS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Polytropic process; Adiabatic process; Acceleration; Shock (circulatory); Scaling; Limit (mathematics); Shock wave; Limiting","score_opus":0.015553872020886051,"score_gpt":0.2583638901860368,"score_spread":0.24281001816515074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032840199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.46787122,0.009082572,0.44305983,0.003973693,0.00051108334,0.00027238484,0.0006558317,0.0014337412,0.073139645],"genre_scores_gemma":[0.96349585,0.0026821888,0.02423567,0.0003232794,0.0004121873,0.00016600276,0.0002906288,0.00026358562,0.008130616],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99915326,0.0003676031,0.000058739923,0.000062879335,0.00018020517,0.00017729837],"domain_scores_gemma":[0.99493885,0.0028645545,0.0008103499,0.0004934761,0.00047386513,0.0004189803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028129488,0.0013526742,0.0016529881,0.0021958726,0.001244803,0.0029475999,0.0021847216,0.002238003,0.0021234793],"category_scores_gemma":[0.020806832,0.0010192115,0.0019326085,0.00090487214,0.0026107123,0.0029769,0.0033780746,0.002460019,0.0005132141],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015308394,0.00012644423,0.0075184708,0.00027698593,0.000113158545,0.0015592946,0.000684977,0.5507613,0.0024644758,0.426861,0.0020410179,0.0074397163],"study_design_scores_gemma":[0.000019474974,0.000012077625,0.00059182063,0.00004331108,0.000015861846,0.00007981403,0.00007486453,0.9389813,0.00019488807,0.059370045,0.0005956322,0.000020907588],"about_ca_topic_score_codex":0.014632737,"about_ca_topic_score_gemma":0.007440421,"teacher_disagreement_score":0.014632737,"about_ca_system_score_codex":0.0017452437,"about_ca_system_score_gemma":0.00089985615,"threshold_uncertainty_score":0.029095113},"labels":[],"label_agreement":null},{"id":"W2032968706","doi":"10.1088/0004-637x/745/2/117","title":"INITIAL CONDITIONS FOR STAR FORMATION IN CLUSTERS: PHYSICAL AND KINEMATICAL STRUCTURE OF THE STARLESS CORE Oph A-N6","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Isothermal process; Fragmentation (computing); Star formation; Deuterium; Spectral line; Line (geometry); Protein filament; Hydrogen; Submillimeter Array","score_opus":0.02056966574686579,"score_gpt":0.29031684826060344,"score_spread":0.26974718251373764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032968706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985594,0.000055829623,0.00019950405,0.000024126908,0.0000013791159,0.000009280875,0.000125769,0.000009574779,0.0010150908],"genre_scores_gemma":[0.9993711,0.000024012596,0.00017165406,0.0000065375443,0.0000023108755,0.0000038724174,0.00022965843,0.0000026214059,0.00018828272],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991274,0.0000063192133,0.000004680633,0.000017264281,0.000026457019,0.000032528726],"domain_scores_gemma":[0.9994873,0.00004812782,0.000085231215,0.000018343566,0.000083544204,0.00027756754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017566314,0.00020536964,0.00024269425,0.00050973846,0.0007149892,0.00076161645,0.00036056718,0.00030780263,0.0016833505],"category_scores_gemma":[0.0008900224,0.00018457342,0.00018384031,0.00019628704,0.00039463522,0.00037670936,0.00092696317,0.00037298191,0.00039034314],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009591739,0.00020620748,0.8760218,0.00007510631,0.00003411477,0.0012589335,0.0009053289,0.00701933,0.10505059,0.003611152,0.00070875883,0.0041494775],"study_design_scores_gemma":[0.000030044223,0.00020150654,0.98560286,0.000013598184,0.0000062404797,0.0003911018,0.0006950988,0.005730345,0.0049126344,0.0015544136,0.0008431416,0.00001902347],"about_ca_topic_score_codex":0.00894606,"about_ca_topic_score_gemma":0.008473285,"teacher_disagreement_score":0.00894606,"about_ca_system_score_codex":0.0008937198,"about_ca_system_score_gemma":0.0004336838,"threshold_uncertainty_score":0.017787993},"labels":[],"label_agreement":null},{"id":"W2032986063","doi":"10.1088/0004-637x/696/1/298","title":"DENSE CORES IN PERSEUS: THE INFLUENCE OF STELLAR CONTENT AND CLUSTER ENVIRONMENT","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Protostar; Star formation; Molecular cloud; Stars; Millimeter; Cluster (spacecraft); Virial theorem; Content (measure theory); Kinetic energy; Galaxy","score_opus":0.011562060694797783,"score_gpt":0.21532489994189316,"score_spread":0.20376283924709537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2032986063","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99967,0.000057811336,0.00002036447,0.0000047940325,4.6844957e-7,7.8726265e-7,0.00005004471,0.0000015943461,0.00019409272],"genre_scores_gemma":[0.99970335,0.000038972736,0.00004105341,0.000005917684,0.0000012605498,7.2662147e-7,0.000098009135,8.402927e-7,0.0001097667],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999639,0.000004437521,0.0000015702198,0.000013101617,0.0000064875276,0.000010574193],"domain_scores_gemma":[0.99987006,0.000020915084,0.0000529328,0.000008653981,0.000014520623,0.000032831605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008030833,0.00016380375,0.000103665436,0.0005217994,0.0001538215,0.00025340437,0.000116232586,0.0000673464,0.00046576883],"category_scores_gemma":[0.00024131747,0.000082073515,0.00006196345,0.00029551133,0.00025357382,0.00013632176,0.0002952151,0.000056496534,0.00010036703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020834591,0.000012574731,0.9824386,0.00001291612,0.000039614155,0.00026671033,0.00036152403,0.0008140938,0.009137853,0.00015850211,0.00011225674,0.006437001],"study_design_scores_gemma":[0.000007690226,0.000033003493,0.99717087,0.0000025487209,0.000007925123,0.0001707137,0.00023292177,0.0005178804,0.0014184931,0.000102310245,0.00033406913,0.0000017319496],"about_ca_topic_score_codex":0.0127924755,"about_ca_topic_score_gemma":0.019000692,"teacher_disagreement_score":0.0127924755,"about_ca_system_score_codex":0.00029541136,"about_ca_system_score_gemma":0.000119839904,"threshold_uncertainty_score":0.025436044},"labels":[],"label_agreement":null},{"id":"W2033057850","doi":"10.1088/0004-637x/769/1/42","title":"FOMALHAUT b: INDEPENDENT ANALYSIS OF THE<i>HUBBLE SPACE TELESCOPE</i>PUBLIC ARCHIVE DATA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; National Research Council Canada; Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Planet; Astrophysics; Astronomy; Spitzer Space Telescope; Spectral energy distribution; Epoch (astronomy); Orbit (dynamics); Telescope; Spectral line; Stars","score_opus":0.0162353550878752,"score_gpt":0.22201393830489896,"score_spread":0.20577858321702375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033057850","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.21758422,0.0011149391,0.103080876,0.0033940757,0.0015679274,0.0007766542,0.6187191,0.030820692,0.022941489],"genre_scores_gemma":[0.35074982,0.00028059195,0.099851586,0.0005407425,0.0006334467,0.0010367804,0.5211995,0.012116499,0.013591049],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9928046,0.0017417157,0.000502223,0.0015517682,0.0021178725,0.0012818233],"domain_scores_gemma":[0.9575281,0.007830297,0.0036799607,0.021155093,0.007770072,0.0020364814],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.012374515,0.001339716,0.00080991903,0.0072940546,0.0021449786,0.002937262,0.003375605,0.0016236138,0.023174247],"category_scores_gemma":[0.043483812,0.0010330904,0.003631883,0.008602268,0.0012546452,0.0025617527,0.0026977204,0.0019708946,0.0144283855],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0041484623,0.0005666516,0.1448417,0.0006948785,0.00237739,0.000467392,0.00057344296,0.0061037885,0.017276494,0.006079589,0.67614937,0.14072089],"study_design_scores_gemma":[0.00089911604,0.00026976876,0.7097366,0.00029477463,0.0014106343,0.00030467493,0.00074013456,0.0356981,0.03236043,0.010678239,0.20719832,0.00040931688],"about_ca_topic_score_codex":0.034250103,"about_ca_topic_score_gemma":0.039079677,"teacher_disagreement_score":0.034250103,"about_ca_system_score_codex":0.0012888518,"about_ca_system_score_gemma":0.0045420025,"threshold_uncertainty_score":0.077525616},"labels":[],"label_agreement":null},{"id":"W2033164039","doi":"10.1088/0004-637x/765/2/84","title":"NON-BAROTROPIC LINEAR ROSSBY WAVE INSTABILITY IN THREE-DIMENSIONAL DISKS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Polytropic process; Barotropic fluid; Rossby wave; Instability; Adiabatic process; Rossby number; Nonlinear system; Linear stability; Perturbation (astronomy); Polytrope","score_opus":0.013998472443795292,"score_gpt":0.23821790989729802,"score_spread":0.22421943745350273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033164039","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9821863,0.00017423791,0.013024112,0.00014287222,0.000010670476,0.00001540507,0.00005813397,0.00011376012,0.0042744633],"genre_scores_gemma":[0.9968966,0.0001013893,0.0022915357,0.000016425662,0.000006985041,0.000018874152,0.00003670197,0.000020393933,0.00061102636],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999604,0.000012506473,0.0000023972086,0.0000050810313,0.000011058859,0.000008543684],"domain_scores_gemma":[0.99984694,0.00006497768,0.00003847767,0.000011741652,0.000019440635,0.00001845288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000112481815,0.00028766363,0.00023737937,0.0002507078,0.00043478113,0.000640704,0.00027678208,0.00032309655,0.0005356991],"category_scores_gemma":[0.00046860872,0.0001571507,0.00027792444,0.00019271897,0.0006395062,0.00030117546,0.00034916753,0.00024205,0.000101404956],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012071744,0.0000771596,0.010010711,0.00009387507,0.000044522007,0.000651177,0.00026889413,0.9256418,0.044941217,0.011690616,0.0004839522,0.0059754886],"study_design_scores_gemma":[0.000018747869,0.000032274264,0.0028701113,0.000003227031,0.0000046532396,0.000059147686,0.000057079844,0.9934617,0.0017801935,0.0014954306,0.00020850386,0.000008932818],"about_ca_topic_score_codex":0.0057235234,"about_ca_topic_score_gemma":0.0026091584,"teacher_disagreement_score":0.0057235234,"about_ca_system_score_codex":0.0004462724,"about_ca_system_score_gemma":0.0003447255,"threshold_uncertainty_score":0.011380434},"labels":[],"label_agreement":null},{"id":"W2033174427","doi":"10.1088/0004-637x/749/2/168","title":"IN SITU FORMATION OF SgrA* STARS VIA DISK FRAGMENTATION: PARENT CLOUD PROPERTIES AND THERMODYNAMICS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Star formation; Stars; Galactic Center; Supermassive black hole; Accretion (finance); Astronomy; Solar mass; Radiative transfer; Galaxy","score_opus":0.020145635227043157,"score_gpt":0.23128398798933208,"score_spread":0.21113835276228893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033174427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99611294,0.00015306895,0.0016158533,0.00007445599,0.000008195452,0.000016041693,0.00015809514,0.000030959767,0.0018304063],"genre_scores_gemma":[0.99899,0.00007607215,0.000573382,0.000016393386,0.0000045744127,0.000009210777,0.00009273175,0.000013520785,0.00022419982],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999027,0.0000246198,0.000005180734,0.000016801865,0.000013611135,0.000037126745],"domain_scores_gemma":[0.99962413,0.00012578898,0.000078539386,0.00003971659,0.000041867865,0.00009002593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003829733,0.00048589124,0.00054229243,0.0003288428,0.0006093886,0.0012088697,0.0009065519,0.0008198375,0.0011333714],"category_scores_gemma":[0.0016067337,0.00029551305,0.0005625788,0.00035208266,0.0006801737,0.0009832231,0.00057391386,0.00037616567,0.00015208508],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022516155,0.00015331403,0.06926205,0.000057953086,0.00012114579,0.00046651662,0.00014480183,0.91426736,0.008270586,0.0041446737,0.0003089478,0.0025775072],"study_design_scores_gemma":[0.00012975225,0.000109209,0.014290155,0.0000087867,0.000037291004,0.00010283982,0.00008455049,0.98149174,0.0020855074,0.0012086941,0.00043522657,0.000016111526],"about_ca_topic_score_codex":0.014294835,"about_ca_topic_score_gemma":0.0066491677,"teacher_disagreement_score":0.014294835,"about_ca_system_score_codex":0.0012420611,"about_ca_system_score_gemma":0.0006302885,"threshold_uncertainty_score":0.02842325},"labels":[],"label_agreement":null},{"id":"W2033278191","doi":"10.1086/504147","title":"The Secular Evolution of Disk Structural Parameters","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":466,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Angular momentum; Instability; Halo; Galaxy; Star formation; Galaxy formation and evolution; Kinematics; Specific relative angular momentum; Thin disk","score_opus":0.0035934667629198905,"score_gpt":0.19086157162905731,"score_spread":0.18726810486613743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033278191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9837177,0.00017875822,0.004404662,0.00029188837,0.000025371713,0.00002003421,0.0014018542,0.00022179348,0.009737954],"genre_scores_gemma":[0.995067,0.00008502447,0.0030973486,0.000056016135,0.000005563571,0.00001823162,0.0008068871,0.00007960701,0.0007842661],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99989784,0.000023233077,0.0000036712838,0.000021415217,0.000027570839,0.00002621966],"domain_scores_gemma":[0.9995371,0.00021435654,0.000061312465,0.00005783574,0.00006432064,0.000064958906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029463193,0.000378884,0.00027721914,0.00048372662,0.0003817846,0.0007024401,0.00064756704,0.000604423,0.002255699],"category_scores_gemma":[0.001790905,0.0002541082,0.0003714791,0.00042776615,0.00047586043,0.0004866335,0.00047934128,0.0005254253,0.00024062958],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004950572,0.000041550466,0.014614319,0.000028365102,0.000049886006,0.00012665708,0.00007396534,0.97354037,0.0036986182,0.0027176095,0.0012995782,0.0037596065],"study_design_scores_gemma":[0.0000136632625,0.000022634715,0.0046135443,0.0000052608693,0.0000064726833,0.000029997622,0.000027350941,0.9932595,0.00083643297,0.0006687275,0.0005065298,0.0000098872615],"about_ca_topic_score_codex":0.01483427,"about_ca_topic_score_gemma":0.0125012845,"teacher_disagreement_score":0.01483427,"about_ca_system_score_codex":0.0007963185,"about_ca_system_score_gemma":0.00062701054,"threshold_uncertainty_score":0.029495895},"labels":[],"label_agreement":null},{"id":"W2033432108","doi":"10.1086/511177","title":"Fluctuations in Babcock‐Leighton Dynamos. II. Revisiting the Gnevyshev‐Ohl Rule","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Dynamo; Physics; Sunspot; Solar dynamo; Amplitude; Solar cycle; Astrophysics; Kinematics; Dynamo theory; Classical mechanics; Magnetic field; Solar wind; Optics; Quantum mechanics","score_opus":0.005747305003988835,"score_gpt":0.2369842914944691,"score_spread":0.23123698649048025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033432108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78698486,0.0011237791,0.18586808,0.0012766941,0.00010793574,0.000027003933,0.0001733715,0.00020835178,0.024229806],"genre_scores_gemma":[0.99607027,0.00016859567,0.0023199974,0.000029337432,0.000020635438,0.000008342522,0.00002425557,0.000020075231,0.0013384676],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990416,0.000027640068,0.0000045843312,0.000023356988,0.000023362714,0.000016929924],"domain_scores_gemma":[0.99972063,0.000095364245,0.00007857874,0.000044225377,0.00002987708,0.000031269043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041766142,0.00023513158,0.00025790706,0.00026856168,0.0002902956,0.00096516305,0.0005504025,0.0004085631,0.0008506731],"category_scores_gemma":[0.0019629942,0.00015802222,0.0002563611,0.00021025084,0.000926624,0.00084884354,0.0004748176,0.00043078206,0.00014026836],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012406998,0.000028696806,0.014534298,0.000046503304,0.000046023546,0.0004969512,0.0004658156,0.3909573,0.0066864504,0.5602356,0.002080427,0.024297781],"study_design_scores_gemma":[0.0000113435435,0.000016759172,0.0033094685,0.0000065353915,0.0000053302733,0.000112638096,0.000047374604,0.8883774,0.00052329205,0.10652288,0.001053011,0.00001390015],"about_ca_topic_score_codex":0.0037374487,"about_ca_topic_score_gemma":0.0021558572,"teacher_disagreement_score":0.0037374487,"about_ca_system_score_codex":0.00052994775,"about_ca_system_score_gemma":0.00021650152,"threshold_uncertainty_score":0.007431388},"labels":[],"label_agreement":null},{"id":"W2033461906","doi":"10.1086/524648","title":"The CO Molecular Outflows of IRAS 16293−2422 Probed by the Submillimeter Array","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Submillimeter Array; Outflow; Physics; Astrophysics; Millimeter; Sky; Redshift; Bipolar outflow; Astronomy; Star formation; Stars; Galaxy; Meteorology","score_opus":0.009539696310652164,"score_gpt":0.2274736516455985,"score_spread":0.21793395533494633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033461906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988926,0.00007221514,0.00013557264,0.000013550884,0.000003393286,0.00000253634,0.0002021977,0.000021276957,0.00065666554],"genre_scores_gemma":[0.99734527,0.00006800985,0.0007041567,0.00003194011,0.000014164394,0.000010572141,0.0014502706,0.000015024208,0.00036059442],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998996,0.000010592952,0.0000034048896,0.000031383155,0.000025640386,0.000029315268],"domain_scores_gemma":[0.99981123,0.00001560502,0.0000725506,0.000020984617,0.000020433903,0.00005928307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017381622,0.0002791465,0.00023092423,0.00045864985,0.00030498233,0.0004730636,0.00022178784,0.00016108435,0.0008051985],"category_scores_gemma":[0.0002946114,0.00019214558,0.0001540296,0.0005387107,0.00012990096,0.00023284928,0.00042097352,0.0003393244,0.00031749488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007917964,0.000289801,0.5765287,0.000094029085,0.00018056779,0.0009269902,0.00083734444,0.0028083925,0.38406837,0.0007575591,0.0018607049,0.030855691],"study_design_scores_gemma":[0.00001388649,0.000059155107,0.99248403,0.000006069336,0.00002017434,0.00016370331,0.000094750256,0.0013899854,0.0039309054,0.00009497064,0.001734209,0.000008204742],"about_ca_topic_score_codex":0.002392335,"about_ca_topic_score_gemma":0.004853823,"teacher_disagreement_score":0.002392335,"about_ca_system_score_codex":0.00019749248,"about_ca_system_score_gemma":0.00012760151,"threshold_uncertainty_score":0.004756868},"labels":[],"label_agreement":null},{"id":"W2033489345","doi":"10.1088/0004-637x/707/2/1809","title":"BLAST OBSERVATIONS OF RESOLVED GALAXIES: TEMPERATURE PROFILES AND THE EFFECT OF ACTIVE GALACTIC NUCLEI ON FIR TO SUBMILLIMETER EMISSION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Active galactic nucleus; Luminous infrared galaxy","score_opus":0.008300452250866466,"score_gpt":0.23549324989634757,"score_spread":0.22719279764548111,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033489345","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99714285,0.00020254735,0.0011198268,0.000035039204,0.000002636455,0.000005672027,0.000556161,0.00006755433,0.0008677626],"genre_scores_gemma":[0.99830425,0.000058659512,0.0008702328,0.000018577166,0.0000042260513,0.0000020936757,0.00054112007,0.000014466049,0.00018635271],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982965,0.00004023758,0.00000874353,0.000054704476,0.000044418815,0.000022240087],"domain_scores_gemma":[0.99908113,0.00025671723,0.00032618007,0.00011328998,0.00008522763,0.00013737664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004948409,0.00019593886,0.00021769693,0.0006046777,0.0001781792,0.000374318,0.00043104106,0.00029061516,0.0007942822],"category_scores_gemma":[0.0009711582,0.00030804952,0.00033083267,0.000657003,0.00018465899,0.00032910594,0.00020399704,0.00028210238,0.00019592169],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029892058,0.00007801379,0.9515323,0.000034083165,0.000110727575,0.0001237065,0.00027931182,0.0030848053,0.03509359,0.0002099742,0.00033932112,0.00881529],"study_design_scores_gemma":[0.000006152131,0.000017334169,0.9962625,0.0000031215443,0.000008521494,0.00004342364,0.000019084195,0.0021573945,0.0013490887,0.000032861455,0.00009667991,0.0000038057526],"about_ca_topic_score_codex":0.009125801,"about_ca_topic_score_gemma":0.025749594,"teacher_disagreement_score":0.009125801,"about_ca_system_score_codex":0.00051836227,"about_ca_system_score_gemma":0.00007666765,"threshold_uncertainty_score":0.018145382},"labels":[],"label_agreement":null},{"id":"W2033499100","doi":"10.1088/0004-637x/794/1/25","title":"PLANET TRAPS AND PLANETARY CORES: ORIGINS OF THE PLANET-METALLICITY CORRELATION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Planet; Exoplanet; Gas giant; Accretion (finance); Jovian; Population; Metallicity; Planetary migration","score_opus":0.006953318244141249,"score_gpt":0.20121857774455615,"score_spread":0.1942652595004149,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033499100","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949185,0.000096757634,0.0036385017,0.00012687815,0.0000021809801,0.0000041203466,0.00012094001,0.00004622513,0.0010458578],"genre_scores_gemma":[0.9996526,0.000020226213,0.0001730869,0.00000763623,0.0000022215747,0.00000226995,0.00003809056,0.0000044687417,0.000099413446],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989676,0.000029214376,0.000006145757,0.00003158147,0.000017736254,0.000018491428],"domain_scores_gemma":[0.9981932,0.00076385256,0.00062096183,0.00020633609,0.00009797697,0.00011772607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031087326,0.00012135347,0.0001729478,0.0004470394,0.00022039801,0.00058826385,0.0004329865,0.00041414378,0.0015400288],"category_scores_gemma":[0.0031796577,0.00012515014,0.00020188924,0.0003868922,0.0006290465,0.00049307523,0.00044157612,0.00026587312,0.00019137474],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034149742,0.00012585719,0.8163298,0.00008766896,0.00011539681,0.00072751864,0.00051081367,0.09151232,0.024689848,0.04845224,0.001128414,0.015978638],"study_design_scores_gemma":[0.000027727543,0.00009776211,0.5365492,0.000012129057,0.000032186235,0.0007960539,0.0002378301,0.4296279,0.0040848297,0.027588014,0.0009216492,0.000024749363],"about_ca_topic_score_codex":0.00251149,"about_ca_topic_score_gemma":0.0019364173,"teacher_disagreement_score":0.00251149,"about_ca_system_score_codex":0.000394801,"about_ca_system_score_gemma":0.00020921118,"threshold_uncertainty_score":0.0051519275},"labels":[],"label_agreement":null},{"id":"W2033509102","doi":"10.1086/588836","title":"On the Connection between Metal Absorbers and Quasar Nebulae","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Quasar; Astrophysics; Physics; Halo; Galaxy; Redshift; OVV quasar; Astronomy; Emission spectrum; Spectral line","score_opus":0.013567080387285706,"score_gpt":0.211987298557822,"score_spread":0.1984202181705363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033509102","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8608463,0.0008714434,0.12016583,0.0034750195,0.00005416865,0.000056633507,0.0003962113,0.0005574898,0.013576801],"genre_scores_gemma":[0.9939721,0.0003636301,0.0034150227,0.00023609881,0.000066607434,0.000018649196,0.000080160295,0.000030078752,0.0018175073],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99987435,0.000029313798,0.000004988022,0.000039273924,0.000017141889,0.000034889803],"domain_scores_gemma":[0.99849474,0.0007634929,0.00035943353,0.00012836167,0.000077477096,0.0001764465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00064096024,0.0004346506,0.0005023417,0.00090093707,0.00053864234,0.0014873297,0.0013474457,0.0011345699,0.0045718434],"category_scores_gemma":[0.0028640523,0.00027450704,0.00044059491,0.0006598199,0.0013507066,0.0018838557,0.00091558194,0.0006382287,0.00079761486],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024276196,0.00024892567,0.25106123,0.00018720284,0.00019078897,0.0019181896,0.0010061905,0.1465261,0.0130679235,0.5450305,0.004384649,0.036135603],"study_design_scores_gemma":[0.000080445636,0.00013785661,0.09884421,0.000042489537,0.00008042254,0.0011930183,0.00023152209,0.4821336,0.0014405706,0.41110215,0.0046383976,0.00007526823],"about_ca_topic_score_codex":0.0033629718,"about_ca_topic_score_gemma":0.0021188415,"teacher_disagreement_score":0.0045718434,"about_ca_system_score_codex":0.0005906519,"about_ca_system_score_gemma":0.00022708841,"threshold_uncertainty_score":0.015294373},"labels":[],"label_agreement":null},{"id":"W2033568523","doi":"10.1086/499940","title":"Constraining Global Properties of the Draco Dwarf Spheroidal Galaxy","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Astronomy; Dwarf galaxy; Dwarf galaxy problem; Milky Way; Dwarf spheroidal galaxy; Dark matter; Dark matter halo; Galaxy; Local Group; Interacting galaxy; Halo","score_opus":0.008336455278282955,"score_gpt":0.19819403185346604,"score_spread":0.1898575765751831,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033568523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997163,0.00003876434,0.0014967296,0.000026871363,0.0000014529969,0.0000029584146,0.000116260606,0.000029063462,0.0011248227],"genre_scores_gemma":[0.99909854,0.000020513377,0.0005548057,0.000006117599,0.0000010557663,0.000001653084,0.00018290401,0.000007291134,0.00012707764],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999316,0.0000166629,0.0000023013283,0.00002234677,0.000008565146,0.00001851346],"domain_scores_gemma":[0.99972636,0.00006742741,0.00006465018,0.000057881232,0.000031249252,0.000052491996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002507092,0.00038612506,0.00032124232,0.00025933993,0.0002487983,0.00072351354,0.00041257308,0.0004004975,0.00067573466],"category_scores_gemma":[0.0010046762,0.00024471182,0.0003998337,0.00030710618,0.00027081306,0.000338118,0.00045664614,0.0003141578,0.0002403606],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012641637,0.000055163902,0.33113083,0.000045119446,0.00013599229,0.00035078675,0.00023849528,0.64399666,0.014780295,0.00384848,0.00040944866,0.004882334],"study_design_scores_gemma":[0.000039421804,0.00008450948,0.107100666,0.000011165718,0.00004778462,0.00015149917,0.00013365292,0.88868254,0.001645282,0.0012493838,0.0008323432,0.000021756341],"about_ca_topic_score_codex":0.019799836,"about_ca_topic_score_gemma":0.021614274,"teacher_disagreement_score":0.019799836,"about_ca_system_score_codex":0.0006285342,"about_ca_system_score_gemma":0.0003846179,"threshold_uncertainty_score":0.039369166},"labels":[],"label_agreement":null},{"id":"W2033690542","doi":"10.1086/517932","title":"The Stellar Mass Tully-Fisher Relation to <i>z</i> = 1.2 from AEGIS","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":225,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Tully–Fisher relation; Physics; Astrophysics; Velocity dispersion; Galaxy; Stellar mass; Redshift; Sigma; Rotation (mathematics); Galaxy rotation curve; Galaxy formation and evolution; Astronomy; Star formation; Geometry; Mathematics","score_opus":0.006084038364981722,"score_gpt":0.2036557012913196,"score_spread":0.19757166292633788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033690542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9609711,0.0010118345,0.018432606,0.0002013591,0.000024637115,0.000024358726,0.0055484236,0.00024857727,0.013536996],"genre_scores_gemma":[0.9879848,0.00020086765,0.005944778,0.00005689236,0.000027783239,0.000019074972,0.004786917,0.000050777027,0.00092812075],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996511,0.000057087273,0.000021746799,0.00013607314,0.00007041503,0.00006368157],"domain_scores_gemma":[0.9990582,0.00017557507,0.0004278533,0.00013022844,0.00012530791,0.00008297653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009786683,0.00037929055,0.00024714827,0.002663617,0.00032580277,0.0006368285,0.0003483433,0.00021460539,0.0018513703],"category_scores_gemma":[0.0028971073,0.0002091998,0.0003169121,0.0011444575,0.00033117665,0.00053977256,0.00070469873,0.0004818017,0.000923262],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004158315,0.000008703925,0.9556117,0.000029426248,0.00005430711,0.000068345165,0.0002347552,0.002832295,0.0018501098,0.005895566,0.0024364213,0.030936759],"study_design_scores_gemma":[0.000004747778,0.00001985529,0.9745272,0.00003308311,0.00002213797,0.00014290288,0.00008729408,0.008569734,0.0011119597,0.006123258,0.0093425,0.000015483267],"about_ca_topic_score_codex":0.017060287,"about_ca_topic_score_gemma":0.013475557,"teacher_disagreement_score":0.017060287,"about_ca_system_score_codex":0.0008527917,"about_ca_system_score_gemma":0.00023579855,"threshold_uncertainty_score":0.033921957},"labels":[],"label_agreement":null},{"id":"W2033721468","doi":"10.1088/0004-637x/718/2/1428","title":"THE YOUNG OUTER DISK OF M83","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Red supergiant; Asymptotic giant branch; Stars; Astronomy; Spiral galaxy; Star formation; Metallicity; Galaxy; Luminosity; Luminosity function; Population; RADIUS; Star cluster; Supergiant","score_opus":0.004536149167652965,"score_gpt":0.20444933480583927,"score_spread":0.1999131856381863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033721468","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99729544,0.00011021295,0.00007762752,0.000019689252,0.000002367459,0.0000039087863,0.00039620756,0.000018836916,0.002075701],"genre_scores_gemma":[0.9969893,0.0001385145,0.00040903888,0.000045650624,0.00000462491,0.000005954188,0.0008684299,0.000010507466,0.0015279792],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999536,0.00000235125,0.000002321175,0.00001389916,0.000010649713,0.000017289307],"domain_scores_gemma":[0.99992335,0.0000053501026,0.000027343287,0.000012604431,0.000011553324,0.00001984166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006714076,0.00015668536,0.00023675192,0.0004006676,0.00061567576,0.0003030072,0.00019574187,0.00026863493,0.0018927627],"category_scores_gemma":[0.00014798979,0.00014342649,0.0001112729,0.00059480895,0.00014756116,0.00016561267,0.00033899027,0.0002062464,0.0015651016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075210305,0.0002486271,0.5582868,0.0000985325,0.000053504515,0.003759069,0.003682841,0.00040586482,0.39063781,0.00065962475,0.0034598424,0.03795535],"study_design_scores_gemma":[0.0000056541894,0.000057030567,0.9932366,0.000004752998,0.0000056304707,0.000820752,0.00023968966,0.00025843846,0.0024915666,0.000045494147,0.0028310881,0.000003406394],"about_ca_topic_score_codex":0.010990021,"about_ca_topic_score_gemma":0.013617075,"teacher_disagreement_score":0.010990021,"about_ca_system_score_codex":0.00041209,"about_ca_system_score_gemma":0.00014421366,"threshold_uncertainty_score":0.021852136},"labels":[],"label_agreement":null},{"id":"W2033814536","doi":"10.1088/0004-637x/725/1/1192","title":"ROTATIONALLY MODULATED<i>g</i>-MODES IN THE RAPIDLY ROTATING δ SCUTI STAR RASALHAGUE (α OPHIUCHI)","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Asteroseismology; Astrophysics; Photometry (optics); Stars; Angular momentum; Amplitude; Parallax; Angular diameter; Astronomy; Classical mechanics; Optics","score_opus":0.009793871662209862,"score_gpt":0.23258286014945886,"score_spread":0.222788988487249,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033814536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996424,0.000044805787,0.000068903806,0.00000810279,7.323791e-7,9.46889e-7,0.000023654513,0.0000049943133,0.00020542921],"genre_scores_gemma":[0.9996375,0.000023005188,0.00015193537,0.00000816666,0.0000017282711,0.0000018333876,0.00007126488,0.0000023067878,0.000102240454],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996257,0.000003422375,0.000002032026,0.0000132634605,0.00000977012,0.000008950864],"domain_scores_gemma":[0.9998677,0.000016993037,0.000057557027,0.000012875722,0.000017705808,0.000027090493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010097065,0.00010705577,0.00010595244,0.0004455757,0.00023954177,0.00029337563,0.00018705774,0.00013825884,0.00026380262],"category_scores_gemma":[0.00025804527,0.0001014897,0.00008261225,0.00026205988,0.000285705,0.00014369095,0.00027196397,0.000202067,0.00008398707],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028264392,0.00008296911,0.72911453,0.000041487783,0.000055229404,0.00041850875,0.00072210794,0.0011803957,0.24540618,0.0003563448,0.0002753778,0.022064244],"study_design_scores_gemma":[0.0000037853645,0.00004215341,0.99615175,0.0000035661415,0.000006209972,0.00012473074,0.00009583295,0.0011499302,0.0020513947,0.00008008273,0.00028580517,0.000004704914],"about_ca_topic_score_codex":0.0027300657,"about_ca_topic_score_gemma":0.0051935622,"teacher_disagreement_score":0.0027300657,"about_ca_system_score_codex":0.00021235317,"about_ca_system_score_gemma":0.00009679901,"threshold_uncertainty_score":0.005428374},"labels":[],"label_agreement":null},{"id":"W2033832621","doi":"10.1088/0004-637x/739/2/101","title":"AN ALUMINUM/CALCIUM-RICH, IRON-POOR, WHITE DWARF STAR: EVIDENCE FOR AN EXTRASOLAR PLANETARY LITHOSPHERE?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Solar System; Exoplanet; Accretion (finance); Mantle (geology); Planetary system","score_opus":0.06932027837992578,"score_gpt":0.31934322104387325,"score_spread":0.2500229426639475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033832621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995254,0.000043950116,0.00003994128,0.00001158431,0.0000012189146,7.4092685e-7,0.000023426606,0.0000027568049,0.000350988],"genre_scores_gemma":[0.999476,0.000029256327,0.00015293999,0.000026425874,0.000002385539,5.2418676e-7,0.00008095947,0.0000019433394,0.00022960917],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999517,0.000003300603,0.0000037791906,0.000015180775,0.000014924626,0.000011046725],"domain_scores_gemma":[0.9998815,0.000008011032,0.000044061057,0.000014747054,0.000016813501,0.000034784465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001106153,0.00017015528,0.0002290079,0.00022587547,0.0003985165,0.00043443227,0.00022723785,0.00027753916,0.0006480705],"category_scores_gemma":[0.00017839544,0.00010544274,0.00010632672,0.00032010715,0.0003447204,0.00020760935,0.00028362285,0.00012511278,0.00026580214],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028272258,0.000031938223,0.83127797,0.00003887191,0.00004109688,0.0014416699,0.00027974113,0.0001559083,0.1622051,0.00021535257,0.00010653113,0.0039230515],"study_design_scores_gemma":[0.000028358043,0.00019909523,0.97654665,0.000009956063,0.000047221074,0.003269853,0.00090533355,0.00066763617,0.015618128,0.0003038974,0.0023965593,0.0000072178204],"about_ca_topic_score_codex":0.003580959,"about_ca_topic_score_gemma":0.009810702,"teacher_disagreement_score":0.003580959,"about_ca_system_score_codex":0.00022609308,"about_ca_system_score_gemma":0.00015680479,"threshold_uncertainty_score":0.0071202517},"labels":[],"label_agreement":null},{"id":"W2033925841","doi":"10.1088/0004-637x/767/1/9","title":"DARK MATTER SUBSTRUCTURE DETECTION USING SPATIALLY RESOLVED SPECTROSCOPY OF LENSED DUSTY GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University","funders":"","keywords":"Substructure; Dark matter; Galaxy; Halo; Cold dark matter; Spectroscopy; Dark matter halo; Gravitational lens","score_opus":0.006925079011249131,"score_gpt":0.2055256608788336,"score_spread":0.19860058186758445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2033925841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974215,0.00007115256,0.0020617186,0.00003511892,9.2636304e-7,0.0000042091433,0.00008681372,0.000020868501,0.000297664],"genre_scores_gemma":[0.9986313,0.000023062412,0.0012242154,0.000006178314,0.0000016124567,0.0000015885149,0.00007010404,0.0000017179807,0.00004027791],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984336,0.000054056858,0.000006173225,0.000041692387,0.00003059317,0.00002398516],"domain_scores_gemma":[0.99878997,0.00047735102,0.00039387602,0.00013311248,0.00008717367,0.00011853933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007066194,0.00027625085,0.0001907544,0.0006504234,0.00020528917,0.0004966401,0.0004348995,0.0002213404,0.0003868697],"category_scores_gemma":[0.0021866227,0.00017970386,0.0003822039,0.00047018012,0.00029579716,0.0006386273,0.00037690403,0.00017473134,0.000055599314],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026369872,0.000118817305,0.7824594,0.00009006402,0.0003566199,0.00027121996,0.00028081602,0.1522705,0.036523465,0.0073799836,0.0002698155,0.019715497],"study_design_scores_gemma":[0.000043587952,0.00025940465,0.41645744,0.000019912179,0.00008680925,0.0001427724,0.00016296087,0.5657564,0.010356384,0.0060856356,0.0005766521,0.000052094165],"about_ca_topic_score_codex":0.010384325,"about_ca_topic_score_gemma":0.011897233,"teacher_disagreement_score":0.010384325,"about_ca_system_score_codex":0.00069849787,"about_ca_system_score_gemma":0.00023845416,"threshold_uncertainty_score":0.020647764},"labels":[],"label_agreement":null},{"id":"W2034005527","doi":"10.1088/0004-637x/750/2/111","title":"DISSIPATIONLESS FORMATION AND EVOLUTION OF THE MILKY WAY NUCLEAR STAR CLUSTER","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":203,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Globular cluster; Star cluster; Supermassive black hole; Milky Way; Solar mass; Merge (version control); Stellar evolution; Star formation; Galactic Center; Spiral galaxy","score_opus":0.009935885742641986,"score_gpt":0.24634726341969518,"score_spread":0.2364113776770532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034005527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972978,0.000058814978,0.0007305607,0.00007217145,0.0000058593637,0.0000058279384,0.00006743961,0.000020040523,0.0017415611],"genre_scores_gemma":[0.998708,0.000033712447,0.00041616993,0.000016079466,0.0000023840762,0.0000053177896,0.000091345544,0.000008163035,0.00071889756],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993706,0.000013105489,0.000002620188,0.000016980186,0.000011706461,0.000018495666],"domain_scores_gemma":[0.99979955,0.000033141598,0.00004603019,0.000023383742,0.000029480823,0.00006846448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015199042,0.00026937484,0.00030667198,0.00027464496,0.00063053396,0.0009453741,0.00088526827,0.0007557981,0.0010800152],"category_scores_gemma":[0.0010205455,0.0002334662,0.0004195393,0.00025588198,0.0007393468,0.0005755131,0.0008587889,0.0003785051,0.0001489481],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020835233,0.00015525245,0.09454726,0.000053941738,0.00012508992,0.00077616086,0.00044335987,0.87816757,0.008054426,0.013659898,0.0007607342,0.0030478768],"study_design_scores_gemma":[0.00008298576,0.0001439601,0.04645334,0.000016749353,0.000041442796,0.00015971536,0.00026081956,0.94685286,0.0012843198,0.0033226437,0.0013473267,0.000033775887],"about_ca_topic_score_codex":0.030395636,"about_ca_topic_score_gemma":0.014690804,"teacher_disagreement_score":0.030395636,"about_ca_system_score_codex":0.0013409083,"about_ca_system_score_gemma":0.00073486485,"threshold_uncertainty_score":0.06043738},"labels":[],"label_agreement":null},{"id":"W2034021253","doi":"10.1088/0004-637x/718/2/920","title":"NEAR-INFRARED THERMAL EMISSION FROM TrES-3b: A<i>Ks</i>-BAND DETECTION AND AN<i>H</i>-BAND UPPER LIMIT ON THE DEPTH OF THE SECONDARY ECLIPSE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Eclipse; Black-body radiation; Physics; Infrared; Radiance; Astrophysics; Wavelength; Astronomy; Radiation; Optics","score_opus":0.008164903632021074,"score_gpt":0.21024930947729256,"score_spread":0.2020844058452715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034021253","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911787,0.00021246573,0.0004933964,0.000068776724,0.000011595208,0.000019425579,0.0008260912,0.00011760302,0.0070719765],"genre_scores_gemma":[0.99640936,0.000086275286,0.0009669998,0.00009382607,0.000015160533,0.000015645808,0.0017265026,0.00004321207,0.0006429063],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998789,0.0000041561843,0.0000027025292,0.000025765528,0.000041156003,0.00004734014],"domain_scores_gemma":[0.99959904,0.000020139862,0.000109654495,0.000026563583,0.00006467499,0.00017997189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013383642,0.00036622194,0.00034184032,0.0005230366,0.00057234144,0.00044139597,0.0003920352,0.0004855528,0.001677506],"category_scores_gemma":[0.00020462529,0.0002590661,0.00047089622,0.00040740627,0.0003257267,0.00019847127,0.00041899353,0.0008510083,0.00068675505],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080611784,0.00017081194,0.19300035,0.0001446872,0.00009697771,0.00090753485,0.0004615121,0.00047284464,0.7929084,0.0002541389,0.0016486013,0.009128155],"study_design_scores_gemma":[0.000037970127,0.00016635042,0.97388655,0.000019037598,0.000032017444,0.00078392564,0.00012364495,0.0012379751,0.021337572,0.000090832305,0.0022690564,0.000015030278],"about_ca_topic_score_codex":0.0064526005,"about_ca_topic_score_gemma":0.014047708,"teacher_disagreement_score":0.0064526005,"about_ca_system_score_codex":0.00044844704,"about_ca_system_score_gemma":0.00020066905,"threshold_uncertainty_score":0.012830079},"labels":[],"label_agreement":null},{"id":"W2034074725","doi":"10.1086/510108","title":"The Mercury‐Manganese Binary Star<i>φ</i>Herculis: Detection and Properties of the Secondary and Revision of the Elemental Abundances of the Primary","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Mercury (programming language); Manganese; Primary (astronomy); Astrophysics; Stars; Physics; Astronomy; Binary star; Binary number; Spectral line; Observatory; Materials science; Metallurgy","score_opus":0.007468295575819384,"score_gpt":0.20396320416041105,"score_spread":0.19649490858459168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034074725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99834573,0.00007000497,0.000033112945,0.000031188658,0.000002400433,0.0000015128085,0.00004064759,0.000013597796,0.0014618773],"genre_scores_gemma":[0.9992067,0.000039615967,0.000112931826,0.000011651083,0.0000037001982,8.921186e-7,0.00012041161,0.0000028936581,0.0005011885],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999959,0.0000030003582,0.0000016515345,0.000014452476,0.000012325964,0.000009557916],"domain_scores_gemma":[0.99989843,0.000006924986,0.000036146906,0.000009029559,0.00002835802,0.000021158388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007403747,0.00014130931,0.00013337219,0.00054800895,0.00049419346,0.0004028762,0.00020797152,0.00022845397,0.0008619645],"category_scores_gemma":[0.00021338831,0.00010874738,0.00003759523,0.00042511997,0.00025753773,0.0001830785,0.0002920946,0.00017170099,0.00022005534],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045871333,0.00009685143,0.47786376,0.00009689929,0.0000200804,0.0018034786,0.00046848768,0.0002896858,0.48302922,0.00096708233,0.0013143523,0.03359139],"study_design_scores_gemma":[0.000022827002,0.00019611776,0.9481747,0.00001063162,0.000015538719,0.0033314861,0.00027164217,0.0010584332,0.040573098,0.00025551344,0.0060816044,0.000008394062],"about_ca_topic_score_codex":0.0042794235,"about_ca_topic_score_gemma":0.0051789633,"teacher_disagreement_score":0.0042794235,"about_ca_system_score_codex":0.00037464738,"about_ca_system_score_gemma":0.00015041803,"threshold_uncertainty_score":0.00850904},"labels":[],"label_agreement":null},{"id":"W2034098787","doi":"10.1086/512800","title":"Cosmological Effects of Powerful AGN Outbursts in Galaxy Clusters: Insights from an<i>XMM‐Newton</i>Observation of MS 0735+7421","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Cooling flow; Galaxy; Galaxy cluster; Metallicity; Cluster (spacecraft); Intracluster medium; Emissivity; Cold front; Redshift; Luminosity; Astronomy","score_opus":0.008303963123907215,"score_gpt":0.22547261020429185,"score_spread":0.21716864708038464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034098787","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99961615,0.000042737858,0.000018695055,0.000014333257,5.120576e-7,8.772718e-7,0.000060354705,0.000004327272,0.00024199256],"genre_scores_gemma":[0.99969184,0.000040840237,0.00006443781,0.00000726497,0.000004208052,9.0667567e-7,0.00012175503,0.000002558239,0.00006628215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.000011148306,0.000004310287,0.000020602603,0.000016740887,0.000018254306],"domain_scores_gemma":[0.9995883,0.000040781168,0.00019475489,0.000026143593,0.000023522962,0.00012663894],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011236603,0.00020151788,0.00020705228,0.0007720091,0.00045076633,0.0005340274,0.00019668591,0.00018964453,0.00070580165],"category_scores_gemma":[0.00047252234,0.000115337614,0.00016380922,0.00064769696,0.0002718232,0.00020920378,0.0004617337,0.0002055883,0.00010882809],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000117835385,0.000035150355,0.97595495,0.000014563437,0.000050570485,0.0004890485,0.00044761432,0.0006094682,0.017289208,0.00015771364,0.00018968155,0.0046443013],"study_design_scores_gemma":[8.2788233e-7,0.000010556326,0.9994049,6.6851777e-7,0.0000074945774,0.00008109774,0.00007269111,0.00015240019,0.00015660694,0.000014871848,0.000095559786,0.0000023576438],"about_ca_topic_score_codex":0.01812011,"about_ca_topic_score_gemma":0.032310307,"teacher_disagreement_score":0.01812011,"about_ca_system_score_codex":0.0005480729,"about_ca_system_score_gemma":0.00019514852,"threshold_uncertainty_score":0.03602928},"labels":[],"label_agreement":null},{"id":"W2034119644","doi":"10.1086/324154","title":"Zirconium to Titanium Ratios in a Large Sample of Galactic S Stars","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Physics; Astrophysics; Zirconium; Barium; Titanium; Abundance (ecology); Spectral line; Astronomy; Metallurgy; Materials science","score_opus":0.01449752226362402,"score_gpt":0.22902136306840118,"score_spread":0.21452384080477716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034119644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99882025,0.00021194646,0.00012575052,0.000014005044,0.0000017602727,0.000005584753,0.00040650932,0.000011499149,0.00040272664],"genre_scores_gemma":[0.9963111,0.00040026027,0.00036179752,0.000044009612,0.00001969249,0.000013486535,0.0019282511,0.00001844252,0.00090302766],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999671,0.00004767182,0.000042363128,0.00011105054,0.00008022827,0.000047849957],"domain_scores_gemma":[0.9994362,0.00010240486,0.00013546093,0.000076999066,0.00013851005,0.000110299006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004312739,0.00032617696,0.00044824337,0.002707107,0.0005077701,0.0006899366,0.00029249812,0.00034780506,0.0013636987],"category_scores_gemma":[0.0012199455,0.00022756046,0.00032197667,0.0014759226,0.00036975916,0.00028393345,0.00056529534,0.00016966341,0.00086693536],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004335926,0.0000710145,0.961138,0.00003579671,0.00013015,0.0002837491,0.0005779741,0.00008150228,0.02388687,0.00010392279,0.00038841055,0.012868979],"study_design_scores_gemma":[0.00001741054,0.00020309718,0.9944976,0.0000032020364,0.00004501692,0.00080913433,0.00024101854,0.00012354832,0.0026231555,0.000044176242,0.0013870392,0.000005520606],"about_ca_topic_score_codex":0.0022599935,"about_ca_topic_score_gemma":0.0027079415,"teacher_disagreement_score":0.002707107,"about_ca_system_score_codex":0.00016067538,"about_ca_system_score_gemma":0.000121695084,"threshold_uncertainty_score":0.0045620203},"labels":[],"label_agreement":null},{"id":"W2034173312","doi":"10.1086/308305","title":"The<i>Hubble Space Telescope</i>Key Project on the Extragalactic Distance Scale. XXIV. The Calibration of Tully‐Fisher Relations and the Value of the Hubble Constant","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":228,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Cepheid variable; Hubble's law; Galaxy; Metallicity; Extinction (optical mineralogy); Cosmic distance ladder; Calibration; Stellar population; Population","score_opus":0.005429901075794139,"score_gpt":0.19644858370145848,"score_spread":0.19101868262566435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034173312","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.06623032,0.05835173,0.07219323,0.03578687,0.013005812,0.0009873845,0.17287612,0.0053378236,0.5752307],"genre_scores_gemma":[0.2774855,0.026346417,0.12649517,0.0034591886,0.0031535223,0.0013152759,0.29902518,0.0010150762,0.26170468],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99935216,0.00011138704,0.00002455144,0.00011373971,0.00026701333,0.00013120884],"domain_scores_gemma":[0.9979102,0.0001518891,0.0004445715,0.00039089995,0.0007223888,0.0003800316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002402045,0.0007914896,0.00042899148,0.002312654,0.00059762294,0.001829764,0.0008714508,0.0007020707,0.014412419],"category_scores_gemma":[0.0023428558,0.00021476261,0.00026728626,0.0026942613,0.0004798764,0.001381072,0.0016507786,0.0013897152,0.011221882],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020835538,0.00008243025,0.018994324,0.00026673736,0.000051112693,0.000059923488,0.0001549651,0.00053388847,0.002725758,0.09035969,0.4545234,0.43203938],"study_design_scores_gemma":[0.000034787765,0.00005815806,0.08399201,0.00015265084,0.000012737978,0.000079272046,0.000074528376,0.0010528855,0.0012013871,0.019641854,0.8936765,0.000023118066],"about_ca_topic_score_codex":0.015280375,"about_ca_topic_score_gemma":0.007971368,"teacher_disagreement_score":0.015280375,"about_ca_system_score_codex":0.002744355,"about_ca_system_score_gemma":0.0019983468,"threshold_uncertainty_score":0.048214376},"labels":[],"label_agreement":null},{"id":"W2034173930","doi":"10.1088/0004-637x/791/2/99","title":"THE MID-INFRARED APPEARANCE OF THE GALACTIC MINI-STARBURST W49A","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Star formation; Galaxy; Stars; Milky Way; Infrared; Molecular cloud; Astronomy","score_opus":0.007503395639647825,"score_gpt":0.2229651979235514,"score_spread":0.21546180228390358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034173930","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986737,0.000056407996,0.00008358772,0.0000147487635,0.0000018902197,0.0000018278369,0.00020907844,0.000011674245,0.0009471378],"genre_scores_gemma":[0.99912876,0.00004149478,0.00015020167,0.000018146442,0.000004254746,0.0000025547358,0.00038218853,0.000004221329,0.00026810044],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997234,0.0000019571894,0.000001957811,0.000009692445,0.0000055643113,0.000008503549],"domain_scores_gemma":[0.99982363,0.000017377592,0.0000843227,0.000014945144,0.00001712994,0.000042701908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004881154,0.00009193733,0.000096593765,0.00039023,0.00017123389,0.00030562445,0.00014877207,0.00021189202,0.0015466175],"category_scores_gemma":[0.0001969368,0.00008107225,0.0001245032,0.00021340193,0.00015028498,0.0001991645,0.00026835283,0.00023947968,0.000421598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023538538,0.000085197215,0.76570344,0.000035496756,0.000047866797,0.0004913246,0.00035094516,0.00020729665,0.22376977,0.0002772576,0.0004909719,0.008305066],"study_design_scores_gemma":[0.000001144488,0.00002142062,0.99885654,0.0000015245054,0.0000037009834,0.00012882252,0.000038320857,0.00007841953,0.00071463274,0.0000113808865,0.0001431519,9.569652e-7],"about_ca_topic_score_codex":0.0018966737,"about_ca_topic_score_gemma":0.0034200067,"teacher_disagreement_score":0.0018966737,"about_ca_system_score_codex":0.00009708188,"about_ca_system_score_gemma":0.00002944838,"threshold_uncertainty_score":0.005173981},"labels":[],"label_agreement":null},{"id":"W2034231150","doi":"10.1086/515564","title":"Supergranulation as an Emergent Length Scale","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Canadian Space Agency","funders":"","keywords":"Physics; Random walk; Polarity (international relations); Magnetic field; Length scale; Magnetic flux; Diffusion; Statistical physics; Scale (ratio); Astrophysics; Mechanics; Quantum mechanics; Statistics","score_opus":0.0061185656346726,"score_gpt":0.24807834880391413,"score_spread":0.24195978316924152,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034231150","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81971616,0.00027348608,0.16686273,0.00070603477,0.00007057234,0.000046722445,0.00015406068,0.00044643309,0.011723807],"genre_scores_gemma":[0.98724735,0.000104802166,0.01078225,0.0000552148,0.000012897433,0.000043746033,0.00005741294,0.000063344305,0.0016329413],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987984,0.000019310706,0.000004889137,0.000029562023,0.000030261623,0.00003610258],"domain_scores_gemma":[0.99950624,0.00015675536,0.00012715397,0.00004868918,0.000057108402,0.00010411412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021635421,0.00025136888,0.00033443893,0.00038719142,0.00055791915,0.0011239895,0.00077071355,0.0007701581,0.0012962099],"category_scores_gemma":[0.0009828424,0.00028022888,0.00057451014,0.00019358697,0.00087713014,0.0012102419,0.000887454,0.00070000696,0.0001470304],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050518058,0.000060224065,0.0042675924,0.000052955747,0.00004057866,0.00040703051,0.0002638529,0.88956285,0.025983162,0.075032055,0.00066203653,0.0036171284],"study_design_scores_gemma":[0.0000095544265,0.00001204921,0.0009510604,0.0000032625192,0.0000050211725,0.000030215628,0.000022518145,0.98582214,0.0007158713,0.011725457,0.00069493626,0.000007923534],"about_ca_topic_score_codex":0.0045555662,"about_ca_topic_score_gemma":0.0023309086,"teacher_disagreement_score":0.0045555662,"about_ca_system_score_codex":0.0013148291,"about_ca_system_score_gemma":0.00061491574,"threshold_uncertainty_score":0.009539843},"labels":[],"label_agreement":null},{"id":"W2034327354","doi":"10.1088/0004-637x/752/2/133","title":"CLASSICAL NOVAE IN ANDROMEDA: LIGHT CURVES FROM THE PALOMAR TRANSIENT FACTORY AND<i>GALEX</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Light curve; Andromeda; Nova (rocket); Galaxy; Milky Way; Andromeda Galaxy; Transient (computer programming); Astronomy; Supernova","score_opus":0.01591784125002053,"score_gpt":0.22483835371141767,"score_spread":0.20892051246139715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034327354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973326,0.00015020142,0.000080589234,0.000016517974,0.0000023397683,0.0000066778243,0.000970128,0.000023054507,0.001417865],"genre_scores_gemma":[0.99705744,0.00006839218,0.0002899946,0.00001607411,0.0000059920217,0.000005667594,0.002237102,0.0000078309595,0.0003116694],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990404,0.000012391925,0.0000071234376,0.000028304466,0.000016687505,0.000031407548],"domain_scores_gemma":[0.9994537,0.00007622419,0.00017212037,0.000065131266,0.00005198703,0.00018083998],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017421113,0.000278093,0.00013227612,0.0013008738,0.000296948,0.00033667102,0.00015494306,0.00021115346,0.0014843463],"category_scores_gemma":[0.00038090517,0.0000889446,0.00018919085,0.00067147013,0.00020917147,0.00017367955,0.00048983353,0.00018727312,0.0004010287],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029328643,0.000046159163,0.9775178,0.000037708443,0.000067469206,0.0003922902,0.00027612952,0.0005278452,0.0071423035,0.00017713592,0.00076303736,0.012758831],"study_design_scores_gemma":[0.0000016423165,0.000017436922,0.99920875,0.0000016394123,0.0000020597183,0.00015891652,0.000033967644,0.00007605479,0.00011326372,0.00001494466,0.00036926693,0.000002121055],"about_ca_topic_score_codex":0.007339101,"about_ca_topic_score_gemma":0.014350338,"teacher_disagreement_score":0.007339101,"about_ca_system_score_codex":0.00031854148,"about_ca_system_score_gemma":0.0000900546,"threshold_uncertainty_score":0.014592767},"labels":[],"label_agreement":null},{"id":"W2034337646","doi":"10.1086/507409","title":"<i>MOST</i>Detects<i>g</i>‐ and<i>p</i>‐Modes in the B Supergiant HD 163899 (B2 Ib/II)","year":2006,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Université du Québec à Montréal; Université de Montréal; Saint Mary's University; University of Toronto; St. Mary's University; University of British Columbia","funders":"","keywords":"Physics; Supergiant; Astrophysics; Asteroseismology; Stars; Radiative transfer; Opacity; Excited state; Amplitude; Light curve; Astronomy; Atomic physics; Optics","score_opus":0.008067583024172738,"score_gpt":0.20525164460784318,"score_spread":0.19718406158367044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034337646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889783,0.00017071281,0.0014027134,0.00008164258,0.000012786584,0.0000081596145,0.0011848874,0.00028317855,0.0078776805],"genre_scores_gemma":[0.9951088,0.000045277153,0.0016423755,0.000060873346,0.000015391735,0.000007818622,0.0017615085,0.000029858978,0.0013281332],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992716,0.0000051436277,0.000003705989,0.000028280618,0.000016826683,0.000018930768],"domain_scores_gemma":[0.99982965,0.0000114135055,0.00004294377,0.000021478878,0.000024035207,0.00007042499],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012974015,0.00014553191,0.00012059259,0.00063579966,0.000261915,0.00030399274,0.00020476484,0.0003140123,0.003957354],"category_scores_gemma":[0.00014945613,0.00015755309,0.00013960572,0.00024431897,0.000120479956,0.00014647291,0.00027773343,0.00015893584,0.0007350466],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037256503,0.000050337785,0.49146456,0.000058365742,0.00006263868,0.00015733883,0.0001241092,0.00019430558,0.48274237,0.00021398067,0.002601262,0.021958193],"study_design_scores_gemma":[0.000005298392,0.000054579625,0.97519726,0.0000053211893,0.000021570579,0.0003543561,0.00005105081,0.0006513083,0.02166743,0.0000486119,0.0019368667,0.000006361922],"about_ca_topic_score_codex":0.002413867,"about_ca_topic_score_gemma":0.006279244,"teacher_disagreement_score":0.003957354,"about_ca_system_score_codex":0.00015502035,"about_ca_system_score_gemma":0.000060009294,"threshold_uncertainty_score":0.013238668},"labels":[],"label_agreement":null},{"id":"W2034365943","doi":"10.1086/318264","title":"Physical Parameters of Erupting Luminous Blue Variables: NGC 2363‐V1 Caught in the Act","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université Laval","funders":"","keywords":"Astrophysics; Physics; Supergiant; Galaxy; Brightness; Astronomy; Large Magellanic Cloud; Ultraviolet; Emission spectrum; Spectral line; Spectroscopy; Absorption spectroscopy; Surface brightness; Stars; Optics","score_opus":0.01454126509681231,"score_gpt":0.2398389650348227,"score_spread":0.22529769993801038,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034365943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987674,0.00004075269,0.000039324088,0.000005656939,7.7965944e-7,0.0000015257509,0.00029238412,0.000004104563,0.00084805104],"genre_scores_gemma":[0.9991961,0.000018643623,0.000070714406,0.0000030697518,0.0000016067446,0.0000013930382,0.00045881356,0.0000033564684,0.00024635094],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998878,0.000010161427,0.000006086651,0.000033555436,0.000030137446,0.000032188647],"domain_scores_gemma":[0.99971646,0.00002498926,0.00011713096,0.00002161022,0.00003162631,0.00008822078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014389977,0.00014539904,0.00016633194,0.001052348,0.0005471629,0.0007234384,0.00021603428,0.00017511261,0.0015674582],"category_scores_gemma":[0.00042522274,0.00007889053,0.00013524065,0.0010352831,0.0004297247,0.00024733733,0.00042341326,0.00022680277,0.00033494373],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006805674,0.000010811451,0.99173963,0.000007670804,0.0000145888835,0.00012210709,0.00046125072,0.00020421647,0.004622724,0.00017094635,0.000110154135,0.002467925],"study_design_scores_gemma":[5.824326e-7,0.000007387709,0.9990583,0.0000012668058,0.0000033340036,0.000144819,0.00014410714,0.00016287733,0.00018289927,0.000017331051,0.0002755456,0.0000014294995],"about_ca_topic_score_codex":0.019907938,"about_ca_topic_score_gemma":0.027803497,"teacher_disagreement_score":0.019907938,"about_ca_system_score_codex":0.0006542413,"about_ca_system_score_gemma":0.00014384146,"threshold_uncertainty_score":0.03958416},"labels":[],"label_agreement":null},{"id":"W2034411092","doi":"10.1086/322246","title":"<i>FUSE</i>Observations of Cooling‐Flow Gas in the Galaxy Clusters A1795 and A2597","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Astrophysics; Physics; Flux (metallurgy); Intracluster medium; Line (geometry); Cooling flow; Galaxy; Emission spectrum; Extinction (optical mineralogy); Atomic physics; Galaxy cluster; Spectral line; Astronomy; Chemistry; Optics","score_opus":0.0184812925799104,"score_gpt":0.22795860070518068,"score_spread":0.20947730812527027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034411092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980319,0.000089923946,0.00009566322,0.000011126539,0.0000038684457,0.0000034783238,0.0004618495,0.000026674057,0.0012754647],"genre_scores_gemma":[0.9982173,0.000043744123,0.000344278,0.000022728307,0.0000096512895,0.0000070379606,0.001098735,0.0000066751104,0.00024987615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999112,0.0000039358515,0.0000066530056,0.00002553687,0.00002361707,0.00002905265],"domain_scores_gemma":[0.99976474,0.000019736799,0.00007631361,0.000028660183,0.00002489026,0.000085667845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010521515,0.00022908213,0.00022166374,0.0012720107,0.0005332365,0.000381158,0.0003741741,0.00031066738,0.0011642261],"category_scores_gemma":[0.00018585751,0.00014025511,0.00029094645,0.00059658545,0.00019161007,0.00018262361,0.00031546515,0.0002020125,0.00025427926],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075407606,0.00016749905,0.7030577,0.0000766577,0.0002699074,0.0016440916,0.0006629655,0.0017533764,0.27447015,0.00074764714,0.0017350095,0.014660956],"study_design_scores_gemma":[0.000011747166,0.00004129403,0.9953709,0.0000052083265,0.000019046396,0.00021524422,0.00007566303,0.00042050754,0.0029004952,0.00007460188,0.00085610023,0.0000090642625],"about_ca_topic_score_codex":0.007817949,"about_ca_topic_score_gemma":0.01021023,"teacher_disagreement_score":0.007817949,"about_ca_system_score_codex":0.00040937075,"about_ca_system_score_gemma":0.000107307606,"threshold_uncertainty_score":0.015544891},"labels":[],"label_agreement":null},{"id":"W2034467386","doi":"10.1088/0004-637x/748/1/3","title":"<i>RXTE</i>OBSERVATIONS OF ANOMALOUS X-RAY PULSAR 1E 1547.0–5408 DURING AND AFTER ITS 2008 AND 2009 OUTBURSTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Pulsar; Flux (metallurgy); Magnitude (astronomy); Static timing analysis; Noise (video); Time derivative","score_opus":0.012967680924602633,"score_gpt":0.27785764841796434,"score_spread":0.2648899674933617,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034467386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960199,0.00007759524,0.00013809676,0.00007878187,0.00001576359,0.00000887036,0.0016845311,0.00006297641,0.0019135199],"genre_scores_gemma":[0.99101865,0.00012852155,0.00096441066,0.00013913045,0.00006857229,0.000029686269,0.006491447,0.00003322324,0.0011265011],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991846,0.0000057341317,0.0000074870954,0.000023411783,0.000022034526,0.000022787372],"domain_scores_gemma":[0.9995733,0.000037260703,0.0002142521,0.00003347898,0.000066697656,0.00007501143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000152924,0.00018929008,0.0002812846,0.00094863673,0.00032225827,0.0003824381,0.0002524316,0.00039949515,0.0008393128],"category_scores_gemma":[0.000440693,0.00009840108,0.00017441907,0.00046235227,0.00017763399,0.00021357455,0.00046365563,0.00044078103,0.0003291254],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060915586,0.00021811183,0.80565214,0.000094387,0.00014589724,0.0011553058,0.00049435307,0.0009939527,0.16402528,0.00033705842,0.005841943,0.0204325],"study_design_scores_gemma":[0.0000052335786,0.00006113673,0.9960639,0.000006211361,0.000015517247,0.00021765495,0.00004876755,0.00027870713,0.0019158578,0.00002198566,0.0013582694,0.0000067267742],"about_ca_topic_score_codex":0.005571544,"about_ca_topic_score_gemma":0.01744394,"teacher_disagreement_score":0.005571544,"about_ca_system_score_codex":0.00023692219,"about_ca_system_score_gemma":0.000137851,"threshold_uncertainty_score":0.0110782385},"labels":[],"label_agreement":null},{"id":"W2034535798","doi":"10.1088/0004-637x/760/1/96","title":"A COOL DUST FACTORY IN THE CRAB NEBULA: A<i>HERSCHEL</i>STUDY OF THE FILAMENTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":194,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Astronomy; Cosmic dust; Nebula; Interstellar medium; Spectral energy distribution; Crab Nebula; Infrared; Galaxy; Stars; Gamma ray","score_opus":0.01831023572081523,"score_gpt":0.23921528682103235,"score_spread":0.22090505110021713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034535798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903488,0.0014127851,0.00078665366,0.00029126625,0.000008593517,0.000008704523,0.00039692412,0.000032182714,0.0067141606],"genre_scores_gemma":[0.99692243,0.000357412,0.0009208288,0.000088710054,0.000019105872,0.000004770618,0.00039490944,0.0000058018313,0.0012859411],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991024,0.000012087753,0.0000029381897,0.000027312826,0.000022313392,0.000025106458],"domain_scores_gemma":[0.99975795,0.000031512493,0.000088325636,0.00003362421,0.000033756933,0.000054855496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021128761,0.00015030835,0.00012020329,0.00036712378,0.00037639614,0.0008086644,0.0002982003,0.00023273299,0.001420096],"category_scores_gemma":[0.00037828108,0.0000925529,0.00012681405,0.00029249841,0.00033231775,0.00043455014,0.00024467098,0.00020460071,0.00024721873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029498758,0.0001027271,0.9212212,0.00009546124,0.00007290517,0.0009900064,0.00038699026,0.0016156627,0.037782796,0.004777653,0.0017722395,0.03088738],"study_design_scores_gemma":[0.000023369012,0.00007030572,0.97888297,0.000042426975,0.00002403183,0.0004691652,0.00025512985,0.0019340472,0.008191631,0.001323992,0.008770713,0.0000123228965],"about_ca_topic_score_codex":0.008394056,"about_ca_topic_score_gemma":0.008603366,"teacher_disagreement_score":0.008394056,"about_ca_system_score_codex":0.00087357825,"about_ca_system_score_gemma":0.0001887242,"threshold_uncertainty_score":0.016690433},"labels":[],"label_agreement":null},{"id":"W2034568322","doi":"10.1088/0004-637x/780/1/40","title":"NON-IDEAL MAGNETOHYDRODYNAMIC SIMULATIONS OF THE TWO-STAGE FRAGMENTATION MODEL FOR CLUSTER FORMATION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Ionization; Fragmentation (computing); Molecular cloud; Drop (telecommunication); Cosmic ray; Extreme ultraviolet; Nonlinear system; Cluster (spacecraft)","score_opus":0.010401161705256071,"score_gpt":0.254398899528625,"score_spread":0.24399773782336892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034568322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9621494,0.00030566572,0.021834474,0.00096003606,0.000080090605,0.00012169737,0.0009228787,0.00020936654,0.013416324],"genre_scores_gemma":[0.9909807,0.00017054845,0.0054835444,0.00013164667,0.00003976441,0.00012619111,0.0004677528,0.000050719667,0.0025490492],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981517,0.00006363768,0.00000875345,0.000025744164,0.00002849804,0.00005828894],"domain_scores_gemma":[0.9989592,0.00045113562,0.00017618376,0.000060816164,0.00010644526,0.00024623994],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042305177,0.00052316143,0.00074384216,0.0006217263,0.0009064625,0.000991943,0.002077313,0.001595401,0.0022551387],"category_scores_gemma":[0.0025558455,0.00046073634,0.00069950946,0.00068630354,0.0012308793,0.00094150973,0.0010916553,0.0010203113,0.00024130433],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000802183,0.000052434843,0.001675876,0.000014457725,0.000020909976,0.00007485352,0.000048187223,0.99354714,0.0004480576,0.0034635859,0.00022076757,0.0003534847],"study_design_scores_gemma":[0.000059367136,0.000014443836,0.00032801676,0.00000188447,0.0000035877272,0.00000738856,0.00001547785,0.9984371,0.0000779937,0.00092440855,0.0001244407,0.0000058221453],"about_ca_topic_score_codex":0.032600556,"about_ca_topic_score_gemma":0.013540331,"teacher_disagreement_score":0.032600556,"about_ca_system_score_codex":0.0015503768,"about_ca_system_score_gemma":0.0009869918,"threshold_uncertainty_score":0.0648216},"labels":[],"label_agreement":null},{"id":"W2034586306","doi":"10.1088/0004-637x/738/2/192","title":"DERIVING THE GLOBAL STRUCTURE OF THE GALACTIC MAGNETIC FIELD FROM FARADAY ROTATION MEASURES OF EXTRAGALACTIC SOURCES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":296,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Sky; Astrophysics; Galactic plane; Halo; Spiral galaxy; Faraday effect; Galactic halo; Disc; Astronomy; Magnetic field; Field (mathematics); Rotation (mathematics); Spiral (railway); Galaxy; Galaxy formation and evolution; Geometry","score_opus":0.012383405588084064,"score_gpt":0.20292343920751696,"score_spread":0.1905400336194329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034586306","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96543735,0.0002593855,0.02716976,0.00003879032,0.0000071242525,0.000027007098,0.0032474324,0.00023589043,0.0035772282],"genre_scores_gemma":[0.98744315,0.00017569966,0.00846116,0.00001239511,0.0000132350315,0.000016642804,0.0035193611,0.000058869642,0.00029959204],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998702,0.000030355848,0.000009524511,0.00005105682,0.000017940978,0.00002080698],"domain_scores_gemma":[0.9994282,0.00015125333,0.00013279116,0.0001329237,0.00009120608,0.00006344335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041344907,0.0006384276,0.0004043581,0.001992468,0.00014071661,0.00059887255,0.00034870463,0.00026722666,0.0016887857],"category_scores_gemma":[0.0018402728,0.00022596357,0.00058852235,0.0011818829,0.00020737412,0.0005232273,0.00057690614,0.00027054982,0.0005213033],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000092971924,0.000056391935,0.81128854,0.00014581635,0.00031978628,0.00020796272,0.0002792763,0.11299734,0.013610691,0.0036383374,0.0010350015,0.05632795],"study_design_scores_gemma":[0.000027248241,0.00009706718,0.90516454,0.00002728272,0.000087233464,0.00012019288,0.00016180123,0.08567064,0.0035888941,0.0028369257,0.0021894882,0.000028756393],"about_ca_topic_score_codex":0.006851362,"about_ca_topic_score_gemma":0.009199633,"teacher_disagreement_score":0.006851362,"about_ca_system_score_codex":0.00037495932,"about_ca_system_score_gemma":0.00025749477,"threshold_uncertainty_score":0.013622999},"labels":[],"label_agreement":null},{"id":"W2034595602","doi":"10.1086/511512","title":"Discovery of New Faint Radio Emission on 8o to 3′ Scales in the Coma Field, and Some Galactic and Extragalactic Implications","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Intergalactic travel; Astronomy; Galaxy; Radio galaxy; Coma Cluster; Cosmic microwave background; Galaxy cluster; Redshift","score_opus":0.010424930853962332,"score_gpt":0.2552965141826127,"score_spread":0.24487158332865033,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034595602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98174137,0.0024484312,0.001923357,0.001139722,0.00021411484,0.000020993373,0.00037849334,0.00011301927,0.012020489],"genre_scores_gemma":[0.99156004,0.00063266366,0.0007022444,0.00029475265,0.00035131158,0.0000064866886,0.00037809883,0.000023826275,0.0060506198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982506,0.0000150637325,0.0000068084564,0.000060057806,0.000034567853,0.000058527814],"domain_scores_gemma":[0.9987148,0.00024308849,0.00025033826,0.0001222903,0.000264613,0.00040479202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047629906,0.00034754787,0.0003893215,0.0012185809,0.0008925663,0.0015284627,0.0006541353,0.0006236679,0.0072895815],"category_scores_gemma":[0.0009549732,0.00028876416,0.00037178412,0.00093609776,0.0010097692,0.0008764768,0.0006200393,0.0005308598,0.0013317436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023463413,0.00035643845,0.61134857,0.00078415306,0.00021265399,0.009670747,0.0020781793,0.000524216,0.25377992,0.0058635576,0.0067317765,0.106303394],"study_design_scores_gemma":[0.000032532567,0.0002387694,0.986922,0.000017285745,0.000040286992,0.0016135798,0.0005157428,0.00015412613,0.004393405,0.0009092366,0.005133727,0.000029337321],"about_ca_topic_score_codex":0.0015391888,"about_ca_topic_score_gemma":0.0021697104,"teacher_disagreement_score":0.0072895815,"about_ca_system_score_codex":0.00033436337,"about_ca_system_score_gemma":0.00014555649,"threshold_uncertainty_score":0.024386108},"labels":[],"label_agreement":null},{"id":"W2034608771","doi":"10.1086/318651","title":"Dust Grain–Size Distributions and Extinction in the Milky Way, Large Magellanic Cloud, and Small Magellanic Cloud","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2620,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Extinction (optical mineralogy); Physics; Astrophysics; Line-of-sight; Interstellar medium; Molecular cloud; Small Magellanic Cloud; Grain size; Albedo (alchemy); Cosmic dust; Particle-size distribution; Astronomy; Galaxy; Stars; Particle size; Optics; Materials science; Geology; Paleontology","score_opus":0.011383460127681311,"score_gpt":0.22949385553949528,"score_spread":0.21811039541181396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034608771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995291,0.000020744332,0.00016012523,0.00000771076,2.044328e-7,0.0000013036027,0.00006761087,0.000011464733,0.00020171754],"genre_scores_gemma":[0.99948066,0.000013906411,0.00020644878,0.0000026089606,9.940867e-7,0.0000013798829,0.00023544926,0.0000056707318,0.000052856],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999101,0.000016865935,0.000005619081,0.000025885885,0.000016165068,0.000025268904],"domain_scores_gemma":[0.9986916,0.00060989574,0.0002960456,0.000115581846,0.00013071834,0.00015610328],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034523953,0.00024520623,0.00017237176,0.0012233141,0.0002096389,0.0004778896,0.0005159365,0.00030599005,0.0006227235],"category_scores_gemma":[0.0018327178,0.00017358882,0.0003462736,0.0007491655,0.00036544105,0.0003962345,0.0003541398,0.0001668555,0.00009702016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032170347,0.000098127384,0.8410686,0.000024354942,0.00010752732,0.00026056042,0.00021580646,0.14251877,0.0068629677,0.0023715803,0.00035371172,0.005796262],"study_design_scores_gemma":[0.00009922876,0.00008690509,0.7839685,0.000009930434,0.000039959396,0.00025821204,0.00016189808,0.2092147,0.0036336237,0.0018946407,0.00060537556,0.00002697442],"about_ca_topic_score_codex":0.01318063,"about_ca_topic_score_gemma":0.01155284,"teacher_disagreement_score":0.01318063,"about_ca_system_score_codex":0.0009463433,"about_ca_system_score_gemma":0.00016623997,"threshold_uncertainty_score":0.026207864},"labels":[],"label_agreement":null},{"id":"W2034701074","doi":"10.1086/587783","title":"Long‐Term Spectroscopic Monitoring of Arcturus","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Line (geometry); Longitude; Stars; Latitude; Emission spectrum; Spectral line; Astronomy","score_opus":0.016190700597746077,"score_gpt":0.24193893221800516,"score_spread":0.2257482316202591,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034701074","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982754,0.00012943243,0.00006401335,0.000029554612,0.000002990466,0.0000051495144,0.00051908015,0.000024855646,0.0009495184],"genre_scores_gemma":[0.998587,0.000074491014,0.00022577254,0.000011987002,0.00000805577,0.0000057071857,0.00083145726,0.0000047145545,0.0002507676],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998124,0.000021071313,0.000011559899,0.00006300687,0.000053250187,0.0000386899],"domain_scores_gemma":[0.99916935,0.000039439838,0.00034442465,0.000049444727,0.00021114419,0.0001861737],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021084647,0.00021920931,0.00024423466,0.0013483448,0.000471784,0.00044620855,0.0003468564,0.00025003296,0.0007214772],"category_scores_gemma":[0.0005565746,0.000120849414,0.00013471322,0.0011256968,0.0001785794,0.00030991095,0.00047980924,0.0002492406,0.00027478536],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009065875,0.00007367701,0.97454774,0.000038699516,0.000055391956,0.00021454395,0.00032950568,0.00032356143,0.009631295,0.000033882032,0.0004458467,0.014215166],"study_design_scores_gemma":[0.0000011357048,0.000028098015,0.99869066,0.000003068638,0.00000651973,0.0000914189,0.00006085562,0.0001748279,0.00039609743,0.0000048638667,0.00054032326,0.0000021673704],"about_ca_topic_score_codex":0.012463226,"about_ca_topic_score_gemma":0.026078168,"teacher_disagreement_score":0.012463226,"about_ca_system_score_codex":0.0005940594,"about_ca_system_score_gemma":0.00021120984,"threshold_uncertainty_score":0.024781346},"labels":[],"label_agreement":null},{"id":"W2034705258","doi":"10.1088/0004-637x/782/2/112","title":"LINEAR COROTATION TORQUES IN NON-BAROTROPIC DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Torque; Planet; Eccentricity (behavior); Planetary system; Protoplanetary disk; Planetary migration; Thermal diffusivity","score_opus":0.00801542927091766,"score_gpt":0.24891514641173348,"score_spread":0.24089971714081582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034705258","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4117677,0.013597309,0.42100015,0.0010188236,0.0007205506,0.00017498955,0.00031101907,0.0010973298,0.15031224],"genre_scores_gemma":[0.97138435,0.0016959329,0.00936459,0.00006200759,0.00015860761,0.000032065185,0.000070842776,0.00017110625,0.017060377],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998759,0.000018037186,0.000008166506,0.000021368398,0.000046700876,0.00002968497],"domain_scores_gemma":[0.99964356,0.000112670874,0.000096728945,0.000045106382,0.000071131486,0.000030746563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017229338,0.0005581452,0.00026716985,0.0006034879,0.00032312764,0.0008155234,0.0007248976,0.00041390577,0.0028343983],"category_scores_gemma":[0.001526952,0.00021922623,0.00042799197,0.0003253716,0.000742825,0.0006985855,0.0008414348,0.00031136122,0.0013662375],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018176729,0.00012691085,0.016490128,0.0010214912,0.000105080515,0.0061289975,0.0016077518,0.3253482,0.10374292,0.41048458,0.0053422926,0.12941988],"study_design_scores_gemma":[0.000031978157,0.000082611725,0.017471308,0.00011311883,0.000049829487,0.0015285145,0.0003600893,0.8692864,0.013933148,0.0837142,0.013351314,0.00007745008],"about_ca_topic_score_codex":0.0028765243,"about_ca_topic_score_gemma":0.002396114,"teacher_disagreement_score":0.0028765243,"about_ca_system_score_codex":0.0007800455,"about_ca_system_score_gemma":0.0003485521,"threshold_uncertainty_score":0.009482026},"labels":[],"label_agreement":null},{"id":"W2034791209","doi":"10.1088/0004-637x/737/1/3","title":"POPULATION PARAMETERS OF INTERMEDIATE-AGE STAR CLUSTERS IN THE LARGE MAGELLANIC CLOUD. II. NEW INSIGHTS FROM EXTENDED MAIN-SEQUENCE TURNOFFS IN SEVEN STAR CLUSTERS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Star cluster; Photometry (optics); Large Magellanic Cloud; Hubble space telescope; Population; Star formation; Galaxy groups and clusters; Stellar population; Star count","score_opus":0.026324375312665616,"score_gpt":0.2651951721225653,"score_spread":0.2388707968098997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034791209","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990809,0.00010413474,0.0004035219,0.00000800093,0.0000010365745,0.0000020703565,0.0000745474,0.000008188341,0.00031752352],"genre_scores_gemma":[0.9994616,0.000030315243,0.00023133938,0.0000032462324,0.0000019835609,0.0000016783446,0.00021547433,0.000005267532,0.000049116803],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999075,0.000007954242,0.000005656174,0.000038072918,0.000015814918,0.000025006433],"domain_scores_gemma":[0.9994667,0.00012222442,0.00015534167,0.000058004385,0.00006238858,0.00013530547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027301328,0.00024810777,0.00025872252,0.0011370525,0.00034026793,0.0006292861,0.0004222166,0.00030428966,0.00079788367],"category_scores_gemma":[0.00084864255,0.00014239628,0.00028165866,0.0005733947,0.00033180966,0.0003918116,0.00046420484,0.0002997766,0.00018818406],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015575122,0.000029200166,0.9682138,0.000026619857,0.00004587478,0.00012702736,0.0005072549,0.009531451,0.012460692,0.0010102766,0.00014567704,0.0077464916],"study_design_scores_gemma":[0.0000061362775,0.00003968036,0.9880283,0.0000040672658,0.000019845225,0.00016243228,0.00020432724,0.009247508,0.00112861,0.00065259874,0.0004971229,0.000009310828],"about_ca_topic_score_codex":0.0043674903,"about_ca_topic_score_gemma":0.0069040214,"teacher_disagreement_score":0.0043674903,"about_ca_system_score_codex":0.00083821215,"about_ca_system_score_gemma":0.00017887678,"threshold_uncertainty_score":0.008684158},"labels":[],"label_agreement":null},{"id":"W2034856282","doi":"10.1086/377074","title":"Dynamical Formation of Close Binary Systems in Globular Clusters","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":345,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Neutron star; Millisecond pulsar; Galaxy; Astronomy; White dwarf; Star cluster; Stars","score_opus":0.007873611728309634,"score_gpt":0.2161334359222449,"score_spread":0.20825982419393527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034856282","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982876,0.00015855774,0.00023605576,0.00002957928,0.0000019028705,0.0000047529115,0.000034965833,0.000008529473,0.0012380558],"genre_scores_gemma":[0.9993753,0.00006266855,0.00013245833,0.0000053077597,0.0000030877209,0.0000024756598,0.00006062308,0.000001391494,0.000356727],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998847,0.0000182051,0.0000056776576,0.00003412438,0.000024933805,0.000032298452],"domain_scores_gemma":[0.99935895,0.00012670022,0.00016581039,0.000038035487,0.000056284793,0.00025420805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020329008,0.00008385727,0.00019461002,0.0005305214,0.0010979647,0.0007053561,0.0002398039,0.0002531045,0.0013029967],"category_scores_gemma":[0.0015354757,0.00015040541,0.000087222914,0.00041101014,0.0005236429,0.0005091934,0.0007518045,0.00016858651,0.0001743617],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021398185,0.00006473785,0.9602866,0.000049683687,0.000053341613,0.00062475563,0.0023989426,0.006155808,0.010452251,0.0077002803,0.0008378839,0.0111617595],"study_design_scores_gemma":[0.00002234063,0.00007968848,0.97915,0.000012733131,0.000030070541,0.0007484069,0.0011135864,0.010698435,0.0011019612,0.004659279,0.0023633773,0.000020097737],"about_ca_topic_score_codex":0.008879694,"about_ca_topic_score_gemma":0.009064023,"teacher_disagreement_score":0.008879694,"about_ca_system_score_codex":0.00069572194,"about_ca_system_score_gemma":0.0002722034,"threshold_uncertainty_score":0.017656028},"labels":[],"label_agreement":null},{"id":"W2034961162","doi":"10.1088/0004-637x/717/2/948","title":"FORMATION OF BLACK HOLE X-RAY BINARIES IN GLOBULAR CLUSTERS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Black hole (networking); Intermediate-mass black hole; Binary number; Mass segregation; Star cluster; Population; Cluster (spacecraft); Binary black hole; Stellar black hole; Stars; Astronomy; Galaxy; Gravitational wave","score_opus":0.009218824893429284,"score_gpt":0.22373476673795475,"score_spread":0.21451594184452547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2034961162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99926585,0.000093927934,0.00023215348,0.0000119077185,0.000002007018,0.0000045974457,0.000017250546,0.000009993222,0.0003622906],"genre_scores_gemma":[0.99952614,0.000057097666,0.00018017394,0.000005989005,0.0000017281149,0.0000026629352,0.000050427938,0.0000023973605,0.00017337357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985623,0.000018205536,0.000007478437,0.00004110721,0.000029000868,0.000047986654],"domain_scores_gemma":[0.999511,0.00009009011,0.0001562938,0.000050130267,0.000033412118,0.00015904194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004203656,0.00028319834,0.00035300403,0.0010608687,0.0009885983,0.0010832874,0.00037488746,0.0004674599,0.0007524775],"category_scores_gemma":[0.0009290414,0.00031799925,0.00019172484,0.00044795635,0.0007736768,0.0004979479,0.00091917434,0.0002490349,0.00021849002],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082944613,0.0001538368,0.8414831,0.00009051968,0.00015136051,0.0011851555,0.0009031893,0.015013601,0.119835444,0.009151716,0.00044434518,0.010758231],"study_design_scores_gemma":[0.00006990715,0.00026325101,0.9196558,0.000017844292,0.00008230786,0.00080038304,0.00074030564,0.03707262,0.033912573,0.0062712226,0.001063641,0.000050047467],"about_ca_topic_score_codex":0.0027714993,"about_ca_topic_score_gemma":0.002386652,"teacher_disagreement_score":0.0027714993,"about_ca_system_score_codex":0.0007395543,"about_ca_system_score_gemma":0.00029465219,"threshold_uncertainty_score":0.0055107474},"labels":[],"label_agreement":null},{"id":"W2035026169","doi":"10.1088/0004-637x/701/1/l12","title":"ON THE ABSENCE OF HIGH METALLICITY-HIGH COLUMN DENSITY DAMPED Lyα SYSTEMS: MOLECULE FORMATION IN A TWO-PHASE INTERSTELLAR MEDIUM","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Metallicity; Interstellar medium; Star formation; Radiation pressure; Ultraviolet; Radiation; Field (mathematics); Extinction (optical mineralogy)","score_opus":0.010262842190023687,"score_gpt":0.2458159351728125,"score_spread":0.23555309298278881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035026169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975998,0.00022454791,0.00085779553,0.000052010244,0.000004761946,0.00000623618,0.00007105738,0.000027980224,0.0011557617],"genre_scores_gemma":[0.9995377,0.000047700756,0.0002239525,0.000018908675,0.0000037384784,0.0000030193116,0.00004850269,0.0000021788953,0.000114306975],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99990785,0.000008026974,0.000008101642,0.000036078985,0.000019279083,0.000020591033],"domain_scores_gemma":[0.9992612,0.00014791462,0.00028148957,0.000103902836,0.00005173657,0.00015383503],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001135067,0.00022448144,0.00025686217,0.00066878233,0.00024834444,0.0008040579,0.00050295907,0.00033370734,0.0030080744],"category_scores_gemma":[0.0005343887,0.00019557378,0.00010263834,0.00033760475,0.00067543914,0.0007504395,0.0006768197,0.00024890836,0.00047214303],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008090035,0.0001337447,0.30912036,0.00024139175,0.00008315,0.00088872627,0.0002969655,0.00078832684,0.6744414,0.0031176435,0.00013543872,0.0099438215],"study_design_scores_gemma":[0.00011604071,0.00036225547,0.8804472,0.000017404336,0.00007263366,0.0030518689,0.0004691004,0.010171155,0.099094786,0.003876166,0.002299011,0.000022353686],"about_ca_topic_score_codex":0.00033346884,"about_ca_topic_score_gemma":0.00042576445,"teacher_disagreement_score":0.0030080744,"about_ca_system_score_codex":0.0001993507,"about_ca_system_score_gemma":0.00009871809,"threshold_uncertainty_score":0.010062993},"labels":[],"label_agreement":null},{"id":"W2035152619","doi":"10.1086/320949","title":"Beryllium in F and G Field Dwarfs from High‐Resolution Canada‐France‐Hawaii Telescope Spectra","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Beryllium; Astronomy; Telescope; Spectral line; Astrophysics; High resolution; Nuclear physics; Remote sensing; Geography","score_opus":0.005711185376140153,"score_gpt":0.193865516692947,"score_spread":0.18815433131680684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035152619","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976041,0.00012889887,0.000109603076,0.000013503831,0.0000015381839,0.000005535168,0.0007506046,0.00001948132,0.0013668002],"genre_scores_gemma":[0.9958503,0.00008412413,0.00049089175,0.000021471633,0.0000021834373,0.000006992419,0.00258486,0.000015086854,0.0009440833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998392,0.0000062730082,0.000007960878,0.000056120552,0.000050768525,0.00003964641],"domain_scores_gemma":[0.9995838,0.000036495858,0.00007781076,0.000037942227,0.00013917591,0.00012484015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002366734,0.00023728027,0.00020374823,0.0017214057,0.0006180583,0.0004581685,0.00028526544,0.00023312695,0.0008708644],"category_scores_gemma":[0.00037997292,0.00018369663,0.00020650457,0.0011116333,0.00022998688,0.00022114045,0.0003299026,0.00013623663,0.0003215012],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002047042,0.00003170259,0.94242966,0.000043327018,0.000080984515,0.00035159572,0.0010436604,0.00034004572,0.04629458,0.0001290343,0.0008245553,0.008226128],"study_design_scores_gemma":[0.0000023276712,0.000008620845,0.99787354,0.0000027880185,0.000009713644,0.000069764574,0.00012403916,0.0001179954,0.0010530776,0.00001085199,0.00072432344,0.0000029334021],"about_ca_topic_score_codex":0.18144114,"about_ca_topic_score_gemma":0.38229766,"teacher_disagreement_score":0.18144114,"about_ca_system_score_codex":0.0015577333,"about_ca_system_score_gemma":0.0003707837,"threshold_uncertainty_score":0.36077005},"labels":[],"label_agreement":null},{"id":"W2035210347","doi":"10.1086/381027","title":"On the Possible Role of Carbon Chains as Carriers of Diffuse Interstellar Bands","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Chemical Physics Studies","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Atomic carbon; Carbon fibers; Spectral line; Carbon chain; Hydrogen; Oscillator strength; Interstellar medium; Atomic physics; Wavelength; Astrophysics; Spectral resolution; Molecular physics; Chemistry; Astronomy; Optics; Materials science; Galaxy; Composite number; Quantum mechanics","score_opus":0.005247815275134298,"score_gpt":0.21852348275382275,"score_spread":0.21327566747868845,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035210347","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6519474,0.04088524,0.008281954,0.05874753,0.015017193,0.00020553508,0.0013106299,0.00035462258,0.22324996],"genre_scores_gemma":[0.81999815,0.02090951,0.0031313084,0.00642754,0.006252582,0.000076760785,0.0014233721,0.0001475988,0.14163314],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996164,0.00006506612,0.000014300301,0.00009568835,0.00011349151,0.000095100106],"domain_scores_gemma":[0.99743265,0.00087933586,0.00019199189,0.00024829348,0.0010456298,0.00020207997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00088243315,0.00040314396,0.000438751,0.0007756948,0.0013480631,0.0018023709,0.0012878672,0.0032541892,0.035702314],"category_scores_gemma":[0.002912278,0.00016903882,0.0003721712,0.0006913537,0.0011333018,0.0024537037,0.0009239536,0.00088366744,0.0056897285],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.007562298,0.00046143733,0.019903613,0.0060652858,0.00043836772,0.007317317,0.0028797782,0.003311895,0.3445428,0.22189572,0.14565846,0.23996301],"study_design_scores_gemma":[0.00047953427,0.0017115606,0.041041624,0.001111595,0.00066937367,0.002941027,0.0053664306,0.005708816,0.18594088,0.18641523,0.5683058,0.0003082237],"about_ca_topic_score_codex":0.00078815286,"about_ca_topic_score_gemma":0.0006311003,"teacher_disagreement_score":0.035702314,"about_ca_system_score_codex":0.00030539228,"about_ca_system_score_gemma":0.00049547054,"threshold_uncertainty_score":0.119436145},"labels":[],"label_agreement":null},{"id":"W2035288312","doi":"10.1086/528838","title":"Spatially Resolved Imaging at 350 μm of Cold Dust in Nearby Elliptical Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Elliptical galaxy; Galaxy; Astronomy; Dust lane; Star formation","score_opus":0.009072276254727316,"score_gpt":0.2062739731729613,"score_spread":0.197201696918234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035288312","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99829954,0.00013324787,0.00045129823,0.000016028453,0.0000012914604,0.0000026190473,0.000105242005,0.000026199781,0.0009643795],"genre_scores_gemma":[0.998384,0.000046932342,0.0010179722,0.000018699258,0.0000042448123,0.0000034812372,0.00013521677,0.0000032393446,0.00038620646],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999629,0.0000020001225,0.0000012908197,0.000010862139,0.000008673135,0.000014218442],"domain_scores_gemma":[0.9999008,0.000012013733,0.000021241252,0.00001069135,0.000013087204,0.000042109936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008053012,0.00009659349,0.00010876533,0.0007134455,0.00021202741,0.00020957734,0.00020042526,0.0001885269,0.0007066392],"category_scores_gemma":[0.0001293387,0.00016390468,0.00009657884,0.00019991356,0.00012721856,0.00012732088,0.0002370494,0.00013245345,0.00018647542],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042094648,0.00007553657,0.13424473,0.00006276431,0.000032840435,0.0010438386,0.00066959864,0.00040272877,0.84526634,0.0005173031,0.0003757532,0.016887592],"study_design_scores_gemma":[0.000009415312,0.00013168795,0.98370475,0.000008883365,0.000022017886,0.00091888435,0.00015218748,0.000591644,0.013303209,0.000108435495,0.0010439105,0.000004961294],"about_ca_topic_score_codex":0.0010436559,"about_ca_topic_score_gemma":0.002177216,"teacher_disagreement_score":0.0010436559,"about_ca_system_score_codex":0.00022075574,"about_ca_system_score_gemma":0.00004875199,"threshold_uncertainty_score":0.0023639798},"labels":[],"label_agreement":null},{"id":"W2035299181","doi":"10.1086/524917","title":"The Frequency of Large‐Radius Hot and Very Hot Jupiters in ω Centauri","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Hot Jupiter; Exoplanet; Astrophysics; Planet; Globular cluster; Stars; Astronomy; Photometry (optics); RADIUS; Orbital period; Transit (satellite)","score_opus":0.010347514668498545,"score_gpt":0.21739090504733263,"score_spread":0.2070433903788341,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035299181","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996265,0.00006262724,0.00003330498,0.000007194722,0.0000011763041,6.4663385e-7,0.0000977369,0.000004074577,0.0001666515],"genre_scores_gemma":[0.9996995,0.000024570374,0.000027372747,0.0000031645216,0.0000031347665,7.945715e-7,0.00015598345,0.0000013611035,0.00008408242],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997991,0.000023629018,0.000012892102,0.000069668866,0.00004174377,0.00005304926],"domain_scores_gemma":[0.99886644,0.00027572954,0.0003873293,0.000113889524,0.00008998206,0.0002665783],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002727817,0.0001503783,0.00017926643,0.0020266415,0.000324246,0.00059293257,0.00025038648,0.00029768248,0.00096789934],"category_scores_gemma":[0.0012772299,0.000112410824,0.00013488211,0.0007498183,0.0005248947,0.00025047676,0.00068867137,0.00016910315,0.00022507871],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007723095,0.0000073438177,0.9928803,0.000008147103,0.000013786266,0.00007198812,0.0003575674,0.00008889533,0.002844991,0.000038247883,0.00007567522,0.003535864],"study_design_scores_gemma":[7.5962936e-7,0.000017005177,0.99934596,0.0000014508065,0.0000051530856,0.00008776213,0.00009230475,0.00007409281,0.00022449155,0.0000133483045,0.0001353268,0.000002259674],"about_ca_topic_score_codex":0.0026694161,"about_ca_topic_score_gemma":0.0037032517,"teacher_disagreement_score":0.0026694161,"about_ca_system_score_codex":0.00022876718,"about_ca_system_score_gemma":0.0000772709,"threshold_uncertainty_score":0.005307734},"labels":[],"label_agreement":null},{"id":"W2035472636","doi":"10.1086/588577","title":"An Improved Magnetic Map of the Milky Way, with the Circularly Orbiting Gas and Magnetic Field Lines Crossing the Dusty Stellar Spiral Arms","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Milky Way; Spiral galaxy; Astrophysics; Galaxy; Astronomy; Pulsar; Circular orbit; Galactic Center","score_opus":0.009622628851700444,"score_gpt":0.20772975751599887,"score_spread":0.19810712866429842,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035472636","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88607895,0.0023637277,0.012589415,0.0035297112,0.00070043147,0.00015526122,0.014789438,0.0033630927,0.07642997],"genre_scores_gemma":[0.95907027,0.00073290284,0.016345346,0.0003465807,0.0009819005,0.000031560157,0.0067318287,0.000287257,0.01547235],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992704,0.0000049189166,0.000003003566,0.000019695324,0.000028144957,0.00001723712],"domain_scores_gemma":[0.9996947,0.000024239465,0.000041184736,0.00003464377,0.000117167176,0.00008811628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011347337,0.00021261573,0.00029345145,0.001575266,0.00038624177,0.00073606335,0.00048031093,0.00063241436,0.011741867],"category_scores_gemma":[0.00053165585,0.00019584138,0.0002101941,0.0011588958,0.00021063529,0.0004945884,0.00056408596,0.0005392802,0.0020655803],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0035021075,0.00044070106,0.117978506,0.0020797958,0.00022073291,0.009282993,0.0020074705,0.015186804,0.40867642,0.010054936,0.06274002,0.36782953],"study_design_scores_gemma":[0.0003430205,0.0003325833,0.83557314,0.00010027469,0.00020332802,0.0045227697,0.00071045884,0.01001867,0.010764267,0.004885796,0.13246426,0.00008141909],"about_ca_topic_score_codex":0.0046066763,"about_ca_topic_score_gemma":0.0074942308,"teacher_disagreement_score":0.011741867,"about_ca_system_score_codex":0.00019868977,"about_ca_system_score_gemma":0.00039139256,"threshold_uncertainty_score":0.039280474},"labels":[],"label_agreement":null},{"id":"W2035542239","doi":"10.1086/592103","title":"The True Shapes of the Dumbbell and the Ring","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Dumbbell; Ring (chemistry); Astronomy; Astrophysics; Medicine","score_opus":0.008710664300587881,"score_gpt":0.20908496870902124,"score_spread":0.20037430440843335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035542239","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94968086,0.00074606796,0.021180976,0.00013625958,0.00005261437,0.000043900207,0.0005252319,0.00027334908,0.027360626],"genre_scores_gemma":[0.98845613,0.00011428701,0.009203926,0.000030010895,0.000008978916,0.000017009295,0.0002691156,0.00006499333,0.0018354917],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997652,0.000024458132,0.000005735385,0.00010051301,0.000050936447,0.00005314869],"domain_scores_gemma":[0.99939394,0.00008141581,0.00009359988,0.0001295042,0.00014922084,0.00015223684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026279973,0.0001991119,0.0001957008,0.00059730175,0.00054972956,0.0015830352,0.00072928786,0.0004010918,0.0028069748],"category_scores_gemma":[0.0020010313,0.00034405704,0.00014204693,0.0003399618,0.0007729333,0.0008315231,0.00066892704,0.00045114997,0.00067444757],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002135015,0.0000996295,0.25200754,0.00040523754,0.00014248026,0.0014799845,0.004200119,0.011880691,0.41460255,0.11832092,0.006916094,0.18780969],"study_design_scores_gemma":[0.00018258908,0.0002908159,0.77317154,0.000121562945,0.00009884431,0.00847252,0.0024529018,0.06417124,0.08135846,0.022343831,0.047033597,0.0003021101],"about_ca_topic_score_codex":0.0035138703,"about_ca_topic_score_gemma":0.0049191457,"teacher_disagreement_score":0.0035138703,"about_ca_system_score_codex":0.0005240479,"about_ca_system_score_gemma":0.00038563876,"threshold_uncertainty_score":0.009390235},"labels":[],"label_agreement":null},{"id":"W2035569671","doi":"10.1086/423197","title":"Hydromagnetic and Gravitomagnetic Crust‐Core Coupling in a Precessing Neutron Star","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Neutron star; Precession; Superfluidity; Pulsar; Coupling (piping); Neutron; Spin (aerodynamics); Core (optical fiber)","score_opus":0.013146753647034992,"score_gpt":0.3024021449654172,"score_spread":0.2892553913183822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035569671","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964233,0.00008895496,0.0012228835,0.00005201231,0.000005261264,0.0000043273853,0.000008108184,0.000016419743,0.002178843],"genre_scores_gemma":[0.9989133,0.000046833833,0.0004559748,0.000019127454,0.0000071552645,0.0000045601937,0.000014032326,0.0000068218997,0.00053212146],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999936,0.0000069362513,0.000003872656,0.000014141048,0.000013900638,0.000025117066],"domain_scores_gemma":[0.9998248,0.000019508885,0.00005865783,0.000017691293,0.0000137093,0.00006561733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012976614,0.00046364497,0.00035124886,0.0003136703,0.00053283334,0.0006539938,0.00045022886,0.00052691734,0.0010909525],"category_scores_gemma":[0.00041590194,0.00024266161,0.00041225168,0.00014446441,0.00096323434,0.00050742977,0.00083217694,0.00033706494,0.00010320265],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007922579,0.00037736743,0.14155145,0.00021185196,0.00023658441,0.008501463,0.0016713827,0.32533148,0.36475128,0.13783285,0.0006681088,0.018073948],"study_design_scores_gemma":[0.00023571998,0.0007047541,0.1317369,0.00002751068,0.00009817307,0.0015859009,0.0005550054,0.8019167,0.015669711,0.045284897,0.0020905046,0.000094230054],"about_ca_topic_score_codex":0.004288933,"about_ca_topic_score_gemma":0.0020807805,"teacher_disagreement_score":0.004288933,"about_ca_system_score_codex":0.0004991245,"about_ca_system_score_gemma":0.00029632528,"threshold_uncertainty_score":0.008527935},"labels":[],"label_agreement":null},{"id":"W2035643958","doi":"10.1086/503022","title":"The Tully‐Fisher Relation in Cluster Cl 0024+1654 at<i>z</i> = 0.4","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Tully–Fisher relation; Physics; Astrophysics; Galaxy rotation curve; Galaxy; Asymmetry; Rotation (mathematics); Luminosity; Kinematics; Cluster (spacecraft); Absolute magnitude; Galaxy formation and evolution; Geometry; Classical mechanics; Mathematics","score_opus":0.004211264042543246,"score_gpt":0.18817361068269683,"score_spread":0.1839623466401536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035643958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988325,0.00005709898,0.00030148667,0.000021257443,0.0000010946397,0.0000014498344,0.000059199796,0.000020643665,0.0007052192],"genre_scores_gemma":[0.9993247,0.000013576206,0.00024757822,0.000007045204,0.0000030347117,0.0000022991226,0.00022115506,0.00000769152,0.00017298623],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996086,0.00007929823,0.000017635019,0.000112090245,0.00008058657,0.000101900994],"domain_scores_gemma":[0.9975915,0.0005772038,0.0009541409,0.00024236673,0.0003464949,0.00028835225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006820529,0.00020028139,0.00023362783,0.0017874924,0.00063126633,0.0006248087,0.00046237477,0.0002930818,0.0011735439],"category_scores_gemma":[0.0049845134,0.0002015223,0.0001750702,0.000891176,0.0006578386,0.0004483594,0.00079480314,0.00032853417,0.00029585892],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009306141,0.000018378225,0.98958194,0.00000865021,0.00003107064,0.000088698594,0.00042078146,0.0019847082,0.0019470195,0.001331838,0.00047549506,0.0040183156],"study_design_scores_gemma":[0.000007135955,0.00002982317,0.99076396,0.000006078663,0.000014167012,0.00008393184,0.00022855241,0.006709222,0.00041461145,0.0010464425,0.00067944056,0.000016614964],"about_ca_topic_score_codex":0.020159716,"about_ca_topic_score_gemma":0.013936164,"teacher_disagreement_score":0.020159716,"about_ca_system_score_codex":0.00073896605,"about_ca_system_score_gemma":0.0003238373,"threshold_uncertainty_score":0.04008478},"labels":[],"label_agreement":null},{"id":"W2035704816","doi":"10.1086/427792","title":"A Survey of O<scp>vi</scp>Absorption in the Local Interstellar Medium","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Local Bubble; Physics; Astrophysics; Absorption (acoustics); Interstellar medium; Stars; White dwarf; Line-of-sight; Optics","score_opus":0.01568040842030464,"score_gpt":0.2463769089084973,"score_spread":0.23069650048819268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035704816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991386,0.00008157125,0.00004026115,0.0000072225994,4.412016e-7,0.0000027941496,0.0003358566,0.000010763694,0.00038242087],"genre_scores_gemma":[0.9983059,0.000104011706,0.00016785655,0.000012712506,0.0000036441324,0.000005767508,0.0011088224,0.0000043441532,0.00028685402],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998523,0.000014157973,0.000007882324,0.000045816487,0.00004016925,0.000039618768],"domain_scores_gemma":[0.9992298,0.000051970128,0.00022216307,0.000037394715,0.00010184091,0.00035680667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002078607,0.00021924693,0.00022254554,0.0015472532,0.0004618191,0.00043371168,0.00022179841,0.00020473401,0.0009172047],"category_scores_gemma":[0.00035549284,0.00010858407,0.00017973318,0.0012515528,0.00020327244,0.00026082475,0.00045161168,0.00013450324,0.00029114375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005087061,0.000023900788,0.98548615,0.000029709658,0.000039408893,0.0001829948,0.00031354598,0.00007990929,0.007347635,0.00003334643,0.00026069098,0.0061518117],"study_design_scores_gemma":[0.000001615265,0.000039055358,0.9987147,0.0000024190763,0.000008489453,0.00012254372,0.00014328971,0.00006881722,0.0003952146,0.000005855681,0.0004962427,0.0000017697412],"about_ca_topic_score_codex":0.010070992,"about_ca_topic_score_gemma":0.023794949,"teacher_disagreement_score":0.010070992,"about_ca_system_score_codex":0.00033118736,"about_ca_system_score_gemma":0.0002755803,"threshold_uncertainty_score":0.020024717},"labels":[],"label_agreement":null},{"id":"W2035725318","doi":"10.1088/0004-637x/747/1/81","title":"RESOLVING THE FAR-IR LINE DEFICIT: PHOTOELECTRIC HEATING AND FAR-IR LINE COOLING IN NGC 1097 AND NGC 4559","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Line (geometry); Galaxy; Photoelectric effect; Starlight; Infrared; Radiation; Ionization; Interstellar medium; Emission spectrum","score_opus":0.013639124064637935,"score_gpt":0.24745057199375858,"score_spread":0.23381144792912065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035725318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990639,0.00005829616,0.0000920874,0.00001203249,0.0000014306067,0.0000025899778,0.000094238116,0.000011721743,0.0006637477],"genre_scores_gemma":[0.99942577,0.000026110141,0.00016978294,0.00001625693,0.0000029585806,0.000003666441,0.0002690309,0.00000612682,0.00008032555],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997805,0.0000167377,0.00001400158,0.00008849524,0.000044543296,0.000055813194],"domain_scores_gemma":[0.9996068,0.0000421335,0.00011007151,0.000050175924,0.000047914375,0.00014290329],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020446147,0.0003159814,0.00035590705,0.0011808544,0.00039060478,0.00059642567,0.00039397163,0.00040514235,0.00076394214],"category_scores_gemma":[0.0006680265,0.00023878951,0.00029160516,0.0004337082,0.00035099013,0.00033884807,0.0007949683,0.00024078909,0.00027088303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017565468,0.00007330699,0.8885091,0.000024491408,0.000081727536,0.00028212045,0.0007030263,0.0005631687,0.102695346,0.00022379095,0.00021691204,0.0064514494],"study_design_scores_gemma":[0.0000047897825,0.000013589161,0.9980696,0.0000033806941,0.000011310875,0.000058526042,0.00015554907,0.0005116506,0.00088861905,0.000042390813,0.0002372148,0.0000034061502],"about_ca_topic_score_codex":0.022323992,"about_ca_topic_score_gemma":0.03112938,"teacher_disagreement_score":0.022323992,"about_ca_system_score_codex":0.00062807725,"about_ca_system_score_gemma":0.00014227779,"threshold_uncertainty_score":0.044388115},"labels":[],"label_agreement":null},{"id":"W2035775267","doi":"10.1088/0004-637x/743/2/107","title":"METAL-POOR LITHIUM-RICH GIANTS IN THE RADIAL VELOCITY EXPERIMENT SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Saint Mary's University","funders":"Science and Technology Facilities Council","keywords":"Red-giant branch; Astrophysics; Giant star; Stars; Physics; Globular cluster; Asymptotic giant branch; Lithium (medication); Halo; Red giant; Metal; Astronomy; Chemistry; Galaxy; Biology","score_opus":0.03924892232414873,"score_gpt":0.2529783212403296,"score_spread":0.21372939891618087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035775267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991916,0.00010220606,0.00007177221,0.000017479344,0.0000014457581,0.0000027482442,0.00034281675,0.00001476027,0.00025515974],"genre_scores_gemma":[0.99778557,0.00008365696,0.00033248824,0.000027572327,0.0000073320584,0.0000052714927,0.0013635416,0.0000055800747,0.0003888948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997975,0.000025833378,0.000013225162,0.00006192662,0.000044118995,0.00005742448],"domain_scores_gemma":[0.999268,0.00006881471,0.00023110252,0.00006336691,0.00008339351,0.00028539286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003658377,0.000263862,0.00024506132,0.0013723779,0.00038075013,0.0003877804,0.00029604064,0.00019393965,0.00066208316],"category_scores_gemma":[0.00065700745,0.0001165729,0.00012546714,0.000781839,0.00022603963,0.00027292347,0.00080296723,0.00013995133,0.00034484646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013314238,0.000019688197,0.99108785,0.000011349289,0.000015511989,0.0002260127,0.00022375736,0.000042507283,0.0039926283,0.0000683554,0.00034956672,0.003829553],"study_design_scores_gemma":[0.0000104115325,0.00005370795,0.9963092,0.000004316125,0.000015248295,0.0006805923,0.00016548941,0.00021138339,0.00065740815,0.00005037212,0.0018359275,0.0000059470176],"about_ca_topic_score_codex":0.0038987154,"about_ca_topic_score_gemma":0.007164277,"teacher_disagreement_score":0.0038987154,"about_ca_system_score_codex":0.0002232473,"about_ca_system_score_gemma":0.000194414,"threshold_uncertainty_score":0.007752061},"labels":[],"label_agreement":null},{"id":"W2035864833","doi":"10.1086/309301","title":"Lensing Effect on the Relative Orientation between the Cosmic Microwave Background Ellipticities and the Distant Galaxies","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Galaxy; Redshift; Universe; Cosmic infrared background; Cosmic background radiation; Amplitude; Background radiation; Cosmology","score_opus":0.009490234291645794,"score_gpt":0.23982395442773044,"score_spread":0.23033372013608464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2035864833","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9725103,0.0016198659,0.008489655,0.00033269185,0.000042649826,0.000018934665,0.0003510078,0.00022083928,0.01641413],"genre_scores_gemma":[0.9983829,0.00024239435,0.00068825367,0.000032377768,0.00002367137,0.0000020957164,0.0000764832,0.000012869311,0.0005390205],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989328,0.00043171935,0.000043171465,0.00022856312,0.00025373665,0.000109917586],"domain_scores_gemma":[0.9927994,0.0039437194,0.0017210327,0.00079319964,0.00035447488,0.0003881273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016142343,0.00063135265,0.00035655723,0.0011341145,0.0003350025,0.0009850698,0.00032406708,0.00036842717,0.004486574],"category_scores_gemma":[0.006770588,0.00030131303,0.00031449014,0.0010620756,0.0011052534,0.0006678037,0.0007068783,0.0005222221,0.00040177317],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015838172,0.00012541858,0.7604115,0.00030681773,0.0007831736,0.00075764226,0.0004440013,0.009112874,0.12159392,0.027609589,0.0012541846,0.076017044],"study_design_scores_gemma":[0.000037687954,0.00014175363,0.9752635,0.000024167308,0.0003209794,0.0006751249,0.00011382926,0.003910848,0.015409516,0.0028748629,0.0011966503,0.000031106785],"about_ca_topic_score_codex":0.0017090013,"about_ca_topic_score_gemma":0.0024930965,"teacher_disagreement_score":0.004486574,"about_ca_system_score_codex":0.00047153223,"about_ca_system_score_gemma":0.00027791277,"threshold_uncertainty_score":0.015009046},"labels":[],"label_agreement":null},{"id":"W2036091709","doi":"10.1086/592739","title":"The Nature of Faint<i>Spitzer</i>‐selected Dust‐obscured Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Spectral energy distribution; Astronomy; Star formation; Luminous infrared galaxy; Luminosity; Photometric redshift","score_opus":0.005215426584973784,"score_gpt":0.19927365117214116,"score_spread":0.19405822458716737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036091709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962664,0.00003256495,0.000050218758,0.000006163699,3.4845547e-7,0.0000015287393,0.00009636389,0.0000052193077,0.0001808409],"genre_scores_gemma":[0.99931633,0.000026471895,0.00009725134,0.000013429985,0.0000027951,0.0000020578193,0.00043624153,0.0000027113317,0.00010282609],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965763,0.00003026344,0.000025470983,0.00011328056,0.0000680303,0.000105289444],"domain_scores_gemma":[0.99876523,0.00014631904,0.00055820495,0.00012714225,0.0001053362,0.00029781353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035070514,0.00026094913,0.00043167596,0.0019250226,0.00042457043,0.00088458735,0.00050756277,0.00028007396,0.00093926437],"category_scores_gemma":[0.0008444654,0.0002394934,0.0002655595,0.0009613938,0.0008090582,0.00049938005,0.000853331,0.00023209523,0.00031279557],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007265407,0.000023774495,0.9910087,0.000009275619,0.000024750108,0.00007598891,0.0002673415,0.00010522212,0.0069250083,0.00006306338,0.000058796162,0.0013653913],"study_design_scores_gemma":[0.0000024461388,0.00002861639,0.99918383,0.000001141492,0.000005192219,0.00012357112,0.00012856325,0.00012930766,0.0002771989,0.000025056295,0.000093291856,0.0000019380766],"about_ca_topic_score_codex":0.0030308045,"about_ca_topic_score_gemma":0.0058518467,"teacher_disagreement_score":0.0030308045,"about_ca_system_score_codex":0.00041163774,"about_ca_system_score_gemma":0.0001436537,"threshold_uncertainty_score":0.0060263276},"labels":[],"label_agreement":null},{"id":"W2036121329","doi":"10.1086/345891","title":"High‐Latitude H<scp>i</scp>in NGC 2613: Buoyant Disk‐Halo Outflow","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Halo; Astrophysics; Physics; Outflow; Galaxy; Buoyancy; Scale height; Thin disk; Plume; Astronomy; Mechanics; Meteorology","score_opus":0.006122309585372631,"score_gpt":0.20208975093320805,"score_spread":0.19596744134783542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036121329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989697,0.000014819143,0.00018909587,0.000010507955,0.0000012434236,0.000003400406,0.00023052008,0.00002449105,0.00055629906],"genre_scores_gemma":[0.9988741,0.00001581968,0.0003091637,0.000008793063,0.0000018316889,0.000003183197,0.00041303918,0.000006884478,0.00036721784],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999621,0.0000024312228,0.0000011781935,0.00001059903,0.0000054521634,0.000018195833],"domain_scores_gemma":[0.99990237,0.0000070578467,0.000027313235,0.0000089989735,0.000006418085,0.00004780529],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059523933,0.00022799025,0.00017865826,0.0002324212,0.00028684724,0.00025359145,0.0002896824,0.00021121025,0.001119976],"category_scores_gemma":[0.00009498515,0.000112683425,0.00014968302,0.00037755026,0.00020275118,0.00007652901,0.0002461629,0.00022586535,0.00036197496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007586327,0.00023190981,0.78295594,0.00008271996,0.00011910856,0.00838891,0.00058887206,0.0069175484,0.1863754,0.0006138344,0.0020325342,0.010934646],"study_design_scores_gemma":[0.000017847864,0.00013763073,0.98619694,0.0000052308396,0.000020204347,0.0009929908,0.00021422678,0.0039551063,0.0075123985,0.00009874804,0.0008374642,0.000011282452],"about_ca_topic_score_codex":0.021853765,"about_ca_topic_score_gemma":0.032081436,"teacher_disagreement_score":0.021853765,"about_ca_system_score_codex":0.00045176066,"about_ca_system_score_gemma":0.00016773574,"threshold_uncertainty_score":0.043453157},"labels":[],"label_agreement":null},{"id":"W2036150081","doi":"10.1086/342527","title":"The Lower Main Sequence and Mass Function of the Globular Cluster Messier 4","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Subdwarf; Physics; Globular cluster; Astrophysics; Luminosity function; Stars; Metallicity; Astronomy; Luminosity; Mass segregation; Cluster (spacecraft); Blue straggler; Population; Proper motion; White dwarf; Galaxy","score_opus":0.01139219439874176,"score_gpt":0.20585069297942069,"score_spread":0.19445849858067893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036150081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99689543,0.000043421856,0.00013194443,0.00004404878,0.0000017190489,0.0000028720478,0.0003881714,0.000028219487,0.0024641086],"genre_scores_gemma":[0.9954406,0.000038289614,0.00027597565,0.000022784912,0.0000064269693,0.0000038781895,0.0011243571,0.000010092747,0.003077561],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999566,0.0000020673783,0.0000016654808,0.000019570569,0.000008882374,0.000011122043],"domain_scores_gemma":[0.99983597,0.000019194154,0.0000521146,0.000014648058,0.00002010504,0.000057940713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009150167,0.00015714335,0.00010329342,0.0008747985,0.00021653167,0.00026821395,0.00018326259,0.00013580357,0.0047715027],"category_scores_gemma":[0.00036078313,0.00005471008,0.0000998424,0.0002001077,0.00018946777,0.00020855674,0.00025877333,0.00012945851,0.0011029462],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003966148,0.000046355723,0.9112134,0.00003535333,0.000045302324,0.0004229801,0.0011891723,0.00075288204,0.054278377,0.0017505107,0.0032718724,0.026597198],"study_design_scores_gemma":[0.0000023243035,0.000026481512,0.99745196,0.0000019952831,0.0000030024014,0.00008177006,0.000043376425,0.0004135776,0.00061258045,0.0000771789,0.0012828242,0.0000028390755],"about_ca_topic_score_codex":0.013674871,"about_ca_topic_score_gemma":0.012252961,"teacher_disagreement_score":0.013674871,"about_ca_system_score_codex":0.00049103756,"about_ca_system_score_gemma":0.00007480598,"threshold_uncertainty_score":0.027190566},"labels":[],"label_agreement":null},{"id":"W2036200883","doi":"10.1086/377493","title":"<i>Far Ultraviolet Spectroscopic Explorer</i>Survey of the Local Interstellar Medium within 200 Parsecs","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Local Bubble; Interstellar medium; Galaxy; Stars; Photoionization; Molecular cloud; Spectral line; Astronomy; Ionization; Ion","score_opus":0.016699981566456912,"score_gpt":0.23623076414878943,"score_spread":0.21953078258233252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036200883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.741723,0.0063693416,0.0073782858,0.006827255,0.0005442131,0.00036289004,0.08487381,0.002636823,0.14928448],"genre_scores_gemma":[0.90179735,0.0019088434,0.009812301,0.0040545575,0.0007141655,0.00019339808,0.05062533,0.00033112097,0.030562945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998884,0.000007971084,0.0000028774446,0.000022290997,0.00003055268,0.00004792655],"domain_scores_gemma":[0.9992987,0.00006580483,0.00014419985,0.00005653984,0.00012600407,0.00030876757],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045128528,0.00025573588,0.00028209484,0.0016663086,0.0007563979,0.00056828605,0.00040868993,0.0005181575,0.0106664905],"category_scores_gemma":[0.0003035363,0.00012441255,0.00030593318,0.0008462282,0.00018526036,0.0006133158,0.0009615949,0.00045858126,0.0022162315],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011858214,0.00044269304,0.47854328,0.00072165206,0.0004404615,0.0017601213,0.00052652176,0.0016923645,0.14416836,0.0058341264,0.22954531,0.13513926],"study_design_scores_gemma":[0.000044358178,0.00019959669,0.9128866,0.00003652519,0.00007441473,0.0004763285,0.00028810144,0.00044944216,0.0051220455,0.0012801962,0.079112254,0.000030177385],"about_ca_topic_score_codex":0.005495476,"about_ca_topic_score_gemma":0.016700812,"teacher_disagreement_score":0.0106664905,"about_ca_system_score_codex":0.00037150018,"about_ca_system_score_gemma":0.00048112386,"threshold_uncertainty_score":0.035682976},"labels":[],"label_agreement":null},{"id":"W2036262191","doi":"10.1088/0004-637x/750/1/33","title":"THE RESOLVED STRUCTURE AND DYNAMICS OF AN ISOLATED DWARF GALAXY: A VLT AND KECK SPECTROSCOPIC SURVEY OF WLM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Galaxy; Stars; Velocity dispersion; Dwarf galaxy; Stellar rotation; RADIUS; Galaxy rotation curve; Astronomy; Galaxy formation and evolution","score_opus":0.006696857053149143,"score_gpt":0.21980110824788215,"score_spread":0.213104251194733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036262191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990953,0.00007430637,0.00009317921,0.000013465806,9.714704e-7,0.0000023497878,0.00035697583,0.000010496577,0.00035287632],"genre_scores_gemma":[0.99828607,0.000055673725,0.00030979136,0.00001621354,0.000004922562,0.000005475163,0.0009597048,0.000007983031,0.00035418238],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985874,0.000012678191,0.000009835252,0.00005468943,0.000025819296,0.000038100916],"domain_scores_gemma":[0.9995772,0.00002239903,0.00016405722,0.00003332227,0.000030487703,0.00017241767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018666344,0.00018303643,0.00027408858,0.001603109,0.00030573635,0.00052871066,0.00028423054,0.00017438729,0.0009520928],"category_scores_gemma":[0.00039436843,0.00012704666,0.00014481087,0.00075736584,0.00026292953,0.00047849063,0.000836474,0.00018123207,0.00042372054],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000073897834,0.00006116636,0.98385715,0.000017120266,0.00003003205,0.00015148729,0.0004298024,0.00015060471,0.005862409,0.00015957639,0.00030094682,0.008905806],"study_design_scores_gemma":[0.0000031840264,0.000042928645,0.9979327,0.00000675737,0.000009196011,0.00018087601,0.000178487,0.00034759854,0.00034741743,0.00005239142,0.00089499913,0.000003608078],"about_ca_topic_score_codex":0.0041697277,"about_ca_topic_score_gemma":0.008769781,"teacher_disagreement_score":0.0041697277,"about_ca_system_score_codex":0.00033591682,"about_ca_system_score_gemma":0.00013073526,"threshold_uncertainty_score":0.0082909465},"labels":[],"label_agreement":null},{"id":"W2036329646","doi":"10.1088/0004-637x/695/1/1","title":"EVIDENCE OF STAR FORMATION IN LOCAL S0 GALAXIES:<i>Spitzer</i>OBSERVATIONS OF THE SAURON SAMPLE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Astronomy; Luminous infrared galaxy; Star formation; Galaxy; Elliptical galaxy; Stellar mass; Interstellar medium","score_opus":0.020603812350254467,"score_gpt":0.23225540822129284,"score_spread":0.21165159587103838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036329646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99909496,0.000057796376,0.00003098566,0.000007325203,4.854792e-7,0.000001549837,0.0001781113,0.0000059963695,0.00062274386],"genre_scores_gemma":[0.9991134,0.000035746343,0.000058084883,0.000008587005,0.000001856206,0.0000021814126,0.0004811465,0.0000021399467,0.00029683797],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986815,0.000013867177,0.000014171585,0.00003934397,0.000027489892,0.000036936348],"domain_scores_gemma":[0.99903154,0.00006666977,0.0003527559,0.00006972647,0.00013845503,0.00034086822],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026085536,0.00017518777,0.0001861198,0.0013642794,0.0003363924,0.0005432322,0.00027922186,0.00017097186,0.0017821081],"category_scores_gemma":[0.00039987886,0.00015331001,0.00018428767,0.0007925025,0.00044339147,0.00024365832,0.0005683221,0.00012741525,0.00043818547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000621855,0.000014274865,0.9933189,0.000015326676,0.000016591412,0.00006492462,0.00026821424,0.000031169955,0.0044762287,0.000038988055,0.000086795604,0.0016063805],"study_design_scores_gemma":[0.0000010605783,0.000016875823,0.99961334,0.0000014887248,0.0000027917902,0.000044118016,0.00006202088,0.000019635365,0.00013205795,0.0000036882573,0.00010223604,7.2136265e-7],"about_ca_topic_score_codex":0.008968858,"about_ca_topic_score_gemma":0.014506756,"teacher_disagreement_score":0.008968858,"about_ca_system_score_codex":0.00028179,"about_ca_system_score_gemma":0.00016565736,"threshold_uncertainty_score":0.017833292},"labels":[],"label_agreement":null},{"id":"W2036350186","doi":"10.1086/344251","title":"SN 1986J VLBI: The Evolution and Deceleration of the Complex Source and a Search for a Pulsar Nebula","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Pulsar; Nebula; Supernova; Surface brightness; Spiral galaxy; RADIUS; Supernova remnant; Flux (metallurgy); Brightness","score_opus":0.024010264094198593,"score_gpt":0.23880770968013637,"score_spread":0.21479744558593777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036350186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998004,0.00027483856,0.00023627334,0.000027919526,0.000002771001,0.000010040548,0.0006646488,0.000015300533,0.0007641809],"genre_scores_gemma":[0.9926208,0.0003871086,0.0013038106,0.000034847453,0.000017486458,0.000014717857,0.0044536237,0.000014840465,0.0011526411],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987566,0.000010028391,0.000008241,0.000028352832,0.000042970532,0.000034736993],"domain_scores_gemma":[0.99969196,0.000018468572,0.00015420576,0.000019910833,0.000042338575,0.000073200834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023963043,0.0002514252,0.00024039658,0.0011185111,0.00040210213,0.00053293747,0.000272686,0.00025500593,0.0006602275],"category_scores_gemma":[0.00044079573,0.00017189888,0.00013768351,0.0010549453,0.00016975436,0.00024741233,0.00040321873,0.0002654023,0.00041784858],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019127024,0.00007721438,0.9723002,0.00003280638,0.000046443445,0.00035078038,0.00021487646,0.0002496117,0.015108525,0.00015537279,0.00039545356,0.010877479],"study_design_scores_gemma":[0.000002126255,0.000016519109,0.9981585,0.0000027794551,0.000006875702,0.00032327813,0.000023643355,0.00024285744,0.00049238134,0.00001566032,0.0007129133,0.0000023799687],"about_ca_topic_score_codex":0.017777959,"about_ca_topic_score_gemma":0.043150228,"teacher_disagreement_score":0.017777959,"about_ca_system_score_codex":0.0005579535,"about_ca_system_score_gemma":0.0002647884,"threshold_uncertainty_score":0.03534895},"labels":[],"label_agreement":null},{"id":"W2036378917","doi":"10.1088/0004-637x/781/2/57","title":"ALL-SKY INTERFEROMETRY WITH SPHERICAL HARMONIC TRANSIT TELESCOPES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":192,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Sky; Interferometry; Astronomical interferometer; Physics; Spherical harmonics; Formalism (music); Spectral density; Telescope; Field of view; Computer science; Optics; Remote sensing; Astronomy; Geology; Telecommunications","score_opus":0.008891542934597227,"score_gpt":0.21270489639296428,"score_spread":0.20381335345836704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036378917","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07743148,0.00012564725,0.9163562,0.00012376322,0.000022712724,0.000030955296,0.00023917948,0.00038725525,0.005282738],"genre_scores_gemma":[0.7193888,0.00015136541,0.27823037,0.000053894208,0.0000334504,0.000029798428,0.0004594409,0.00010701474,0.0015458653],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99968195,0.00008301741,0.000012912074,0.00006130025,0.00012612047,0.000034845252],"domain_scores_gemma":[0.9995265,0.000116783485,0.00009704043,0.000178633,0.000053853586,0.000027284123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007677287,0.00043272533,0.00022816402,0.000505273,0.00035227113,0.00087879656,0.00071498606,0.0002924814,0.0012250826],"category_scores_gemma":[0.0020103124,0.0002551436,0.0005332934,0.00089627673,0.00062627596,0.0013124014,0.0012977571,0.0005178546,0.00028831218],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003365328,0.000070924216,0.03858241,0.00015856567,0.00023557515,0.00050960155,0.00085282774,0.27780804,0.07654657,0.45766282,0.0027214026,0.1445147],"study_design_scores_gemma":[0.000021523429,0.00009347407,0.017512297,0.000018068436,0.000035493747,0.00037206657,0.00014881916,0.8576585,0.015634015,0.09490098,0.013561019,0.00004371768],"about_ca_topic_score_codex":0.0026193,"about_ca_topic_score_gemma":0.004610804,"teacher_disagreement_score":0.0026193,"about_ca_system_score_codex":0.00082117063,"about_ca_system_score_gemma":0.0006787459,"threshold_uncertainty_score":0.0059580803},"labels":[],"label_agreement":null},{"id":"W2036501057","doi":"10.1086/320248","title":"Constraints on Stirring and Dissipation of MHD Turbulence in Molecular Clouds","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Magnetohydrodynamics; Dissipation; Molecular cloud; Turbulence; Supersonic speed; Flux (metallurgy); Star formation","score_opus":0.009739124023100152,"score_gpt":0.24636295578952,"score_spread":0.23662383176641985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036501057","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9690748,0.0017825294,0.022703387,0.00044646356,0.000034229997,0.00002499007,0.00020289063,0.00014650573,0.00558422],"genre_scores_gemma":[0.9981598,0.00038185067,0.0012452912,0.000012011035,0.000020719668,0.000009562272,0.0000822494,0.000014585728,0.00007387787],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99966633,0.000050026298,0.00003381277,0.000059816568,0.00009020953,0.00009979658],"domain_scores_gemma":[0.9919652,0.0057253474,0.001190174,0.0005537194,0.00026235834,0.00030314407],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013313022,0.0009999465,0.0005611353,0.0008656012,0.00091195613,0.0019818584,0.0010397369,0.0006976015,0.0011805294],"category_scores_gemma":[0.013669123,0.0005076063,0.0004593379,0.00047734487,0.0011914405,0.002824315,0.0017366675,0.00094185787,0.00025210308],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002668417,0.00028388912,0.2625713,0.0006854525,0.00022166045,0.0013801196,0.001035863,0.21911165,0.3178133,0.15307657,0.00069566665,0.04045606],"study_design_scores_gemma":[0.00022715314,0.0005623681,0.11469447,0.0001393744,0.00013729568,0.0005278883,0.00028461704,0.6988471,0.10614912,0.07525773,0.0029629983,0.00020988187],"about_ca_topic_score_codex":0.0010415456,"about_ca_topic_score_gemma":0.0006261751,"teacher_disagreement_score":0.0019818584,"about_ca_system_score_codex":0.00080051523,"about_ca_system_score_gemma":0.0002152624,"threshold_uncertainty_score":0.0070406795},"labels":[],"label_agreement":null},{"id":"W2036564741","doi":"10.1086/591082","title":"On Using the <i>WMAP</i> Distance Information in Constraining the Time-evolving Equation of State of Dark Energy","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"","keywords":"CMB cold spot; Dark energy; Cosmic microwave background; Physics; Astrophysics; Energy (signal processing); Spectral density; Equation of state; Cosmology; Statistics; Quantum mechanics; Mathematics","score_opus":0.01021899868996865,"score_gpt":0.22687599670758882,"score_spread":0.21665699801762017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036564741","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.43768612,0.016910436,0.46553546,0.012058861,0.0010734076,0.00015438886,0.003657714,0.0006278494,0.06229577],"genre_scores_gemma":[0.7923315,0.013230623,0.18636233,0.0016812115,0.0012264836,0.0000764066,0.0030077035,0.0002585929,0.0018251588],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99908566,0.00037172355,0.000032511736,0.00013086622,0.0003219617,0.0000573108],"domain_scores_gemma":[0.9869064,0.008640581,0.0013756526,0.0017215045,0.0010609791,0.00029489663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0045850957,0.001322514,0.00075554056,0.0026421554,0.00084696914,0.0028962947,0.0010795817,0.0011187504,0.0021304777],"category_scores_gemma":[0.027387803,0.00048308956,0.0006182003,0.002700606,0.0025318926,0.0070332456,0.0036927282,0.0019663584,0.00044980142],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010160658,0.00012791535,0.046664607,0.0010904539,0.0006492785,0.00057133596,0.000752552,0.17842157,0.013385043,0.4342599,0.008486169,0.31457502],"study_design_scores_gemma":[0.00011803141,0.00024405078,0.025911586,0.00075192255,0.0002975794,0.00047673334,0.0005028618,0.31638208,0.014278417,0.61499655,0.025792807,0.00024734298],"about_ca_topic_score_codex":0.0045203157,"about_ca_topic_score_gemma":0.0036890074,"teacher_disagreement_score":0.0045850957,"about_ca_system_score_codex":0.0006492034,"about_ca_system_score_gemma":0.00073733967,"threshold_uncertainty_score":0.0242486},"labels":[],"label_agreement":null},{"id":"W2036632043","doi":"10.1088/0004-637x/748/1/36","title":"RADIO MONITORING OF THE TIDAL DISRUPTION EVENT SWIFT J164449.3+573451. I. JET ENERGETICS AND THE PRISTINE PARSEC-SCALE ENVIRONMENT OF A SUPERMASSIVE BLACK HOLE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Supermassive black hole; Flattening; Lorentz factor; RADIUS; Jet (fluid); Black hole (networking); Milky Way; Very Long Baseline Array","score_opus":0.009834807780060108,"score_gpt":0.21776806134446056,"score_spread":0.20793325356440046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036632043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990453,0.00007144042,0.00011960118,0.00001657047,0.000007346344,0.0000067181572,0.00020653309,0.000015365775,0.0005111617],"genre_scores_gemma":[0.9980464,0.00007313249,0.00049549225,0.000022424312,0.000032947435,0.000011117663,0.0008955665,0.000005940809,0.00041687745],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992967,0.0000057879947,0.0000047180083,0.000017720877,0.000019352894,0.000022703443],"domain_scores_gemma":[0.99962044,0.000038069466,0.00013504806,0.00003287325,0.000078847246,0.00009467934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018451431,0.00023172131,0.00021527759,0.000850982,0.00029505894,0.00029006044,0.00026056677,0.00033020656,0.0007452729],"category_scores_gemma":[0.00040823087,0.00011025483,0.00015552716,0.00041345914,0.00017867121,0.00019027249,0.00032341306,0.00028830062,0.00027614055],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008553415,0.00026017101,0.816374,0.0000818129,0.0001069101,0.0018448051,0.00041573108,0.0008866283,0.14578988,0.00019654946,0.0011484063,0.032039747],"study_design_scores_gemma":[0.000009101792,0.00014594832,0.99622416,0.000004697495,0.000021197,0.00025429332,0.000042637294,0.00046979502,0.001786811,0.000019274523,0.001016321,0.000005664435],"about_ca_topic_score_codex":0.0030744986,"about_ca_topic_score_gemma":0.0073875254,"teacher_disagreement_score":0.0030744986,"about_ca_system_score_codex":0.0002217815,"about_ca_system_score_gemma":0.000112043,"threshold_uncertainty_score":0.006113231},"labels":[],"label_agreement":null},{"id":"W2036809080","doi":"10.1088/0004-637x/784/1/8","title":"UTILITY OF GALAXY CATALOGS FOR FOLLOWING UP GRAVITATIONAL WAVES FROM BINARY NEUTRON STAR MERGERS WITH WIDE-FIELD TELESCOPES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Science and Technology Facilities Council","keywords":"Physics; LIGO; Gravitational wave; Galaxy; Sky; Neutron star; Astrophysics; Astronomy; Galaxy merger; Binary number; Telescope; Star formation","score_opus":0.011375806479832612,"score_gpt":0.2898489218879014,"score_spread":0.2784731154080688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036809080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8122468,0.0019170748,0.14242539,0.0005597144,0.00010726115,0.0005982198,0.016541282,0.011604805,0.013999429],"genre_scores_gemma":[0.88658637,0.0004338878,0.097057834,0.000082550694,0.000046466575,0.00012396087,0.013814486,0.00025425223,0.0016001475],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987728,0.00036491101,0.00009899374,0.00025593047,0.0003804983,0.00012691123],"domain_scores_gemma":[0.9792773,0.0053613256,0.0028666626,0.006638195,0.004726614,0.0011298623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0058337743,0.00051147334,0.0005580245,0.007929141,0.0007362029,0.002286106,0.001026306,0.0005887426,0.0019062081],"category_scores_gemma":[0.021197358,0.00042368055,0.0004908055,0.004184622,0.00032602338,0.0027189548,0.001315067,0.0004203229,0.001436668],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043073684,0.00019200082,0.67506003,0.00018879586,0.0001959975,0.00025968495,0.00048249832,0.023669116,0.00637379,0.006182107,0.007217834,0.27974734],"study_design_scores_gemma":[0.00012307097,0.00047722302,0.60629714,0.0003222033,0.00039915784,0.0008056292,0.000935628,0.3070049,0.025615683,0.011721222,0.046032894,0.00026539204],"about_ca_topic_score_codex":0.014834721,"about_ca_topic_score_gemma":0.01659577,"teacher_disagreement_score":0.014834721,"about_ca_system_score_codex":0.0010152637,"about_ca_system_score_gemma":0.0013102582,"threshold_uncertainty_score":0.030852318},"labels":[],"label_agreement":null},{"id":"W2036815187","doi":"10.1088/0004-637x/780/1/11","title":"CXOGBS J173620.2-293338: A CANDIDATE SYMBIOTIC X-RAY BINARY ASSOCIATED WITH A BULGE CARBON STAR","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; National Science Foundation; University of California, Los Angeles; Jet Propulsion Laboratory","keywords":"Bulge; Astrophysics; Physics; Luminosity; Astronomy; Carbon star; Gravitational lens; Stars; Galactic plane; Star (game theory); Population; Galaxy; Redshift","score_opus":0.0072017944332101475,"score_gpt":0.19637382439874915,"score_spread":0.189172029965539,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036815187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99618113,0.00014136647,0.00011703341,0.00017076235,0.0000141904,0.000017567614,0.0004189533,0.000015028569,0.0029240986],"genre_scores_gemma":[0.9966683,0.00010931538,0.000413473,0.00012385956,0.000031342595,0.000007736183,0.0012213279,0.000011056013,0.001413514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999249,0.00000409376,0.0000036893784,0.000018977651,0.000018583083,0.000029748886],"domain_scores_gemma":[0.99981695,0.0000076138936,0.0000428921,0.000004903931,0.000009409761,0.00011826625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008719547,0.00040710403,0.00029036537,0.0008654292,0.0011879095,0.00065535615,0.00046189214,0.0005056669,0.0038056727],"category_scores_gemma":[0.0001393218,0.00013175647,0.00011055751,0.00086869136,0.0003798695,0.00023199478,0.0006407538,0.00031499003,0.0006427507],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005447337,0.00026492207,0.9004612,0.00011548517,0.000038208433,0.044506352,0.0007577878,0.0004832692,0.035721328,0.002226935,0.0050316784,0.009848181],"study_design_scores_gemma":[0.00005828003,0.00016272407,0.9641975,0.000046345314,0.00002911206,0.020711713,0.001163996,0.0019751121,0.0020770102,0.0006748264,0.008881409,0.00002200079],"about_ca_topic_score_codex":0.012314982,"about_ca_topic_score_gemma":0.041031428,"teacher_disagreement_score":0.012314982,"about_ca_system_score_codex":0.00047121546,"about_ca_system_score_gemma":0.00029555164,"threshold_uncertainty_score":0.024486601},"labels":[],"label_agreement":null},{"id":"W2036829516","doi":"10.1088/0004-637x/752/1/2","title":"IONIZED NITROGEN AT HIGH REDSHIFT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Redshift; Plateau de Bure Interferometer; Astrophysics; Galaxy; Interstellar medium; Ionization; Star formation; Astronomy","score_opus":0.01076040119523833,"score_gpt":0.23282524775374017,"score_spread":0.22206484655850184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036829516","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967372,0.00016183869,0.00036078066,0.000029659988,0.0000028084255,0.000002468576,0.00012452001,0.000040173498,0.0025405427],"genre_scores_gemma":[0.99913245,0.00005191662,0.0003178526,0.000022200746,0.0000045210477,0.0000030807769,0.00016912156,0.000003973377,0.00029473222],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998565,0.0000060787916,0.0000027605597,0.00006187702,0.000030237896,0.000042535365],"domain_scores_gemma":[0.99983656,0.000011646636,0.00008002589,0.00001294333,0.000015844182,0.000042951273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010648125,0.00023177169,0.00017576301,0.00061682635,0.00038357012,0.000570198,0.00040163053,0.0002557327,0.0011820856],"category_scores_gemma":[0.00022655897,0.00017192609,0.00008527996,0.0005122171,0.00029175254,0.00030068343,0.0006613469,0.0002670723,0.00028696022],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036696153,0.00007986712,0.75914377,0.00007920162,0.000112335474,0.0014782501,0.0008524112,0.001111844,0.20579581,0.0032940148,0.0009724329,0.02671311],"study_design_scores_gemma":[0.000016958335,0.000050821396,0.9855671,0.000008791787,0.00003185388,0.00063694303,0.00016112684,0.0012507185,0.007542219,0.0006209437,0.0041005,0.000012095374],"about_ca_topic_score_codex":0.005781085,"about_ca_topic_score_gemma":0.0072896816,"teacher_disagreement_score":0.005781085,"about_ca_system_score_codex":0.0006723012,"about_ca_system_score_gemma":0.00012725266,"threshold_uncertainty_score":0.011494875},"labels":[],"label_agreement":null},{"id":"W2036857553","doi":"10.1086/517491","title":"Millihertz Quasi‐periodic Oscillations from Marginally Stable Nuclear Burning on an Accreting Neutron Star","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Neutron star; Physics; Astrophysics; Accretion (finance); Oscillation (cell signaling); Luminosity; Stars; Galaxy","score_opus":0.014169294483991813,"score_gpt":0.24109208302936871,"score_spread":0.2269227885453769,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036857553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99476385,0.00006943609,0.0031236159,0.000060066894,0.00000545688,0.000003874008,0.000018104904,0.00003642939,0.001919176],"genre_scores_gemma":[0.9990575,0.000039661987,0.0006085342,0.0000070397073,0.000005022629,0.0000040551126,0.000017384538,0.000011769308,0.00024899602],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99996316,0.000009275274,0.0000017079986,0.000005607537,0.000009803288,0.0000105197],"domain_scores_gemma":[0.9998191,0.00006625412,0.000058976322,0.000014405818,0.00001026272,0.000030988132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016322406,0.00033884068,0.00021392039,0.00020106703,0.00044866852,0.00049421185,0.00033083296,0.00032214064,0.0011542086],"category_scores_gemma":[0.0006145059,0.00020179532,0.00038765938,0.0001845106,0.00052521174,0.00039310646,0.0005128004,0.0004194483,0.0001220812],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006640906,0.00023637984,0.07857381,0.00017107051,0.00015531528,0.0027581588,0.00084973563,0.7558687,0.10039506,0.04483327,0.0007256791,0.0147687225],"study_design_scores_gemma":[0.000037626676,0.000087346496,0.032100253,0.000006640109,0.000019996454,0.00017869669,0.0000867445,0.95601773,0.0043485067,0.006742104,0.00035749754,0.000016914846],"about_ca_topic_score_codex":0.002192536,"about_ca_topic_score_gemma":0.0012226263,"teacher_disagreement_score":0.002192536,"about_ca_system_score_codex":0.0006299051,"about_ca_system_score_gemma":0.00016069852,"threshold_uncertainty_score":0.0045703053},"labels":[],"label_agreement":null},{"id":"W2036888129","doi":"10.1088/0004-637x/714/1/778","title":"A<i>SPITZER</i>SURVEY OF PROTOPLANETARY DISK DUST IN THE YOUNG SERPENS CLOUD: HOW DO DUST CHARACTERISTICS EVOLVE WITH TIME?","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Serpens; Astrophysics; Physics; Young stellar object; Silicate; Spectral energy distribution; Protostar; Spectral line; Stars; Circumstellar dust; Astronomy; Molecular cloud; Infrared; Redshift; Galaxy; Star formation","score_opus":0.008398134378271168,"score_gpt":0.21320232676620254,"score_spread":0.20480419238793138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036888129","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990766,0.00021545566,0.000056066092,0.000016315884,9.225602e-7,0.0000020730263,0.0003609022,0.0000066104258,0.0002650372],"genre_scores_gemma":[0.9979144,0.00039929416,0.0003059984,0.000017818362,0.000011372429,0.000003912816,0.0010459223,0.000003582926,0.00029776647],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994683,0.0000073346655,0.0000048385787,0.000014366098,0.000010789056,0.000015752228],"domain_scores_gemma":[0.9994912,0.00005781709,0.0002863288,0.000031579977,0.000056456112,0.00007660586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014058076,0.0002020433,0.00012585513,0.00141151,0.00015670643,0.00032672752,0.00012236813,0.00012620592,0.0006185327],"category_scores_gemma":[0.0004487083,0.00006945604,0.00013224383,0.00078566436,0.00017026305,0.00021554294,0.0001593688,0.00009419708,0.00027813407],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045416746,0.00001660486,0.9908302,0.000011003669,0.000018734194,0.00007466363,0.00009265095,0.00009544571,0.002804495,0.000013629507,0.00010777104,0.0058895],"study_design_scores_gemma":[5.999014e-7,0.000024550971,0.99919397,0.0000021014073,0.0000056891063,0.00008195873,0.00004598525,0.00008503647,0.00027341107,0.000008181554,0.0002776388,8.510306e-7],"about_ca_topic_score_codex":0.0065796906,"about_ca_topic_score_gemma":0.0106556425,"teacher_disagreement_score":0.0065796906,"about_ca_system_score_codex":0.0001965097,"about_ca_system_score_gemma":0.000120439756,"threshold_uncertainty_score":0.013082802},"labels":[],"label_agreement":null},{"id":"W2036995529","doi":"10.1088/0004-637x/754/1/68","title":"LUMINOSITIES OF BARRED AND UNBARRED S0 GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Luminosity; Galaxy; Elliptical galaxy; Lenticular galaxy; Peculiar galaxy; Asymmetry; Spiral galaxy; Disc; Bulge","score_opus":0.007715887540306764,"score_gpt":0.2069424499753087,"score_spread":0.19922656243500192,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2036995529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99746764,0.00016345434,0.00017910497,0.000007715027,0.000002391609,0.0000030176627,0.00015116954,0.000046820405,0.0019786325],"genre_scores_gemma":[0.9985719,0.000056621324,0.00020480453,0.000014797103,0.0000050645003,0.0000037760203,0.00046738796,0.00001176067,0.0006638882],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971265,0.000032474796,0.00004048509,0.00008086403,0.00005737625,0.000076181284],"domain_scores_gemma":[0.9980556,0.00039858324,0.0006576953,0.00016699609,0.0001938691,0.0005273251],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000563911,0.0002554252,0.00028835644,0.0035761187,0.0002674076,0.0011795801,0.00044113497,0.00036333434,0.005152193],"category_scores_gemma":[0.0015247421,0.0002842593,0.00031153698,0.0011256514,0.00073462294,0.00065131544,0.000892534,0.0002872156,0.0012223813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030383084,0.000038880844,0.96483564,0.000044719156,0.00006901999,0.00008017569,0.0007147461,0.00020696236,0.023628993,0.00047631064,0.00015601107,0.009444772],"study_design_scores_gemma":[0.0000027697274,0.000030882973,0.99840766,0.0000054612274,0.000008592142,0.000085220956,0.00012998746,0.00017851354,0.000856443,0.00007432551,0.00021541449,0.0000047767594],"about_ca_topic_score_codex":0.0016491705,"about_ca_topic_score_gemma":0.0015024758,"teacher_disagreement_score":0.005152193,"about_ca_system_score_codex":0.00030562154,"about_ca_system_score_gemma":0.00007671394,"threshold_uncertainty_score":0.017235816},"labels":[],"label_agreement":null},{"id":"W2037299008","doi":"10.1088/0004-637x/731/1/77","title":"ERRATUM: “MULTI-WAVELENGTH OBSERVATIONS OF THE FLARING GAMMA-RAY BLAZAR 3C 66A IN 2008 OCTOBER” (2011, ApJ, 726, 43)","year":2011,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Blazar; Astrophysics; Wavelength; Astronomy; Gamma ray; Optics","score_opus":0.02746436329208864,"score_gpt":0.22677803460479753,"score_spread":0.19931367131270888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037299008","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0015822946,0.0013906556,0.0002767282,0.03991881,0.92957133,0.00004026558,0.006557241,0.00066759746,0.01999505],"genre_scores_gemma":[0.02303497,0.0062108296,0.0029893075,0.063685775,0.12707585,0.0001235496,0.02518192,0.0018165752,0.7498811],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99899536,0.00007947429,0.00020344701,0.00015765248,0.000436647,0.00012738287],"domain_scores_gemma":[0.99571973,0.00066014036,0.00048056108,0.000378412,0.0024105608,0.00035055762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009486285,0.002412825,0.0013067612,0.0038251649,0.0035997613,0.0032768224,0.0019181034,0.0038245197,0.05191708],"category_scores_gemma":[0.008104115,0.00074738206,0.0011884477,0.0018982512,0.0011528763,0.002062665,0.0016180705,0.004046365,0.03923365],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009207118,0.000016276377,0.0002730441,0.00008033785,0.000009726449,0.0002862425,0.000018251169,0.000045158766,0.0001607584,0.00032923254,0.9956049,0.003083954],"study_design_scores_gemma":[0.00004878786,0.000060636463,0.007975832,0.00027486403,0.000049046215,0.00041505785,0.000159223,0.00018902932,0.0006908131,0.0006908233,0.9893975,0.0000483638],"about_ca_topic_score_codex":0.02827152,"about_ca_topic_score_gemma":0.059887502,"teacher_disagreement_score":0.05191708,"about_ca_system_score_codex":0.0028651922,"about_ca_system_score_gemma":0.0031147893,"threshold_uncertainty_score":0.17367995},"labels":[],"label_agreement":null},{"id":"W2037390816","doi":"10.1086/320569","title":"A Submillimeter View of Star Formation near the H<scp>ii</scp>Region KR 140","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"James Clerk Maxwell Telescope; Physics; Astrophysics; Bolometer; Submillimeter Array; Stars; Molecular cloud; Star formation; Mass distribution; Telescope; Astronomy; Galaxy; Optics","score_opus":0.016159127987660466,"score_gpt":0.23363951217440754,"score_spread":0.21748038418674706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037390816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9748489,0.00018070392,0.0011136297,0.00010396686,0.000009803862,0.000014969334,0.0017916751,0.00026831502,0.021668166],"genre_scores_gemma":[0.9944364,0.00013791928,0.002041121,0.00006093296,0.000025119558,0.000007147871,0.0010854034,0.000029165358,0.002176796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997854,0.0000010688036,6.621914e-7,0.000005263757,0.00000701937,0.0000073539845],"domain_scores_gemma":[0.9998938,0.000015518344,0.000026314747,0.0000092644295,0.000012842506,0.000042193857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000039244747,0.00008547894,0.00006732425,0.00063555245,0.00017366001,0.00021641342,0.00015462161,0.00012440934,0.0056829075],"category_scores_gemma":[0.00008197567,0.000100784026,0.00013530774,0.0003053061,0.00007946132,0.00015624017,0.000276342,0.00025250454,0.00075677934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034589236,0.00015689248,0.5813483,0.00015287503,0.0001087736,0.0021857223,0.001275643,0.0021528602,0.3423549,0.0016203641,0.011101035,0.057196792],"study_design_scores_gemma":[0.0000059479235,0.000036163492,0.99285454,0.000008375719,0.000010965685,0.0005343377,0.00013120659,0.001012834,0.0015461072,0.00007190262,0.0037845166,0.0000030785172],"about_ca_topic_score_codex":0.005863187,"about_ca_topic_score_gemma":0.010015476,"teacher_disagreement_score":0.005863187,"about_ca_system_score_codex":0.00017578278,"about_ca_system_score_gemma":0.0001074857,"threshold_uncertainty_score":0.01901126},"labels":[],"label_agreement":null},{"id":"W2037392005","doi":"10.1086/324298","title":"Multiple Peaks in the Angular Power Spectrum of the Cosmic Microwave Background: Significance and Consequences for Cosmology","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":351,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Reionization; Amplitude; Spectral density; Spectral index; Cosmology; Robustness (evolution); Adiabatic process; Parameter space; Cosmic variance; Cosmic background radiation; COSMIC cancer database; Astrophysics; Maximization; Statistics; Statistical physics; Mathematics; Spectral line; Redshift; Quantum mechanics","score_opus":0.014360081956582215,"score_gpt":0.23826569276526618,"score_spread":0.22390561080868396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037392005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8502794,0.026113579,0.030063182,0.012429602,0.001669016,0.000020788695,0.0018992054,0.001031681,0.07649356],"genre_scores_gemma":[0.9859365,0.004269286,0.0021698067,0.000258916,0.0007738249,0.0000060256402,0.0003851654,0.00012938166,0.006071207],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998047,0.00004210713,0.000010271689,0.000064377375,0.000061462386,0.000017152073],"domain_scores_gemma":[0.99873906,0.0006614788,0.00021142939,0.0001405745,0.00013236668,0.00011505361],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051786815,0.0002851961,0.0003109794,0.0013697715,0.000308145,0.0022446774,0.00027617923,0.00039478045,0.007788602],"category_scores_gemma":[0.0043178806,0.00018303416,0.000149266,0.0019258774,0.00065617805,0.0007820622,0.00052806875,0.000374697,0.001448734],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007033123,0.00010239357,0.27097452,0.00040167442,0.00030962113,0.0024582464,0.0008583412,0.006857604,0.019913722,0.04641511,0.05456006,0.59644544],"study_design_scores_gemma":[0.000065547196,0.00013124269,0.8322413,0.00022284358,0.0002199946,0.007135746,0.0010203705,0.017929826,0.007188167,0.08351847,0.050223123,0.00010323563],"about_ca_topic_score_codex":0.00058731035,"about_ca_topic_score_gemma":0.00059173856,"teacher_disagreement_score":0.007788602,"about_ca_system_score_codex":0.00025161586,"about_ca_system_score_gemma":0.0001302706,"threshold_uncertainty_score":0.026055455},"labels":[],"label_agreement":null},{"id":"W2037430951","doi":"10.1086/427729","title":"Selection Effects in the Redshift Distribution of Gamma-Ray Bursts and Associated Quasi-stellar Objects and Active Galaxies","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Carleton University","funders":"","keywords":"Physics; QSOS; Redshift; Astrophysics; Galaxy; Gamma-ray burst; Astronomy; Cosmic distance ladder; Active galactic nucleus","score_opus":0.0057363552816590705,"score_gpt":0.21736481450848455,"score_spread":0.21162845922682547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037430951","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99650085,0.00020583584,0.0018436689,0.000022415652,0.0000027163724,0.0000066648527,0.00008577274,0.000031806423,0.0013003191],"genre_scores_gemma":[0.99948585,0.000045273016,0.00026327718,0.000004173298,0.0000046642454,0.000002411621,0.00009651291,0.000005811166,0.00009202145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99927443,0.00024127577,0.00006244597,0.00017369047,0.00013348616,0.000114680166],"domain_scores_gemma":[0.9866781,0.0065989615,0.0039908383,0.0017124533,0.0005815554,0.00043804848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015321289,0.00022011848,0.00023541981,0.0019416633,0.00027238514,0.0011997118,0.0002977347,0.00045094255,0.0019830982],"category_scores_gemma":[0.009724204,0.00022200173,0.00027763416,0.0015786603,0.0013095033,0.0006701027,0.0005408757,0.000277568,0.00039566227],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038246487,0.000023174725,0.9749429,0.000025582602,0.00005875209,0.0002608853,0.00044989926,0.0014966967,0.0055621676,0.0033122045,0.00010828044,0.013376895],"study_design_scores_gemma":[0.0000146912635,0.000060781847,0.99134237,0.000008432582,0.000029251582,0.0008232455,0.00019011156,0.0034616804,0.0015207729,0.0022442741,0.00029029165,0.000014187373],"about_ca_topic_score_codex":0.0008084922,"about_ca_topic_score_gemma":0.00093073543,"teacher_disagreement_score":0.0019830982,"about_ca_system_score_codex":0.0005465958,"about_ca_system_score_gemma":0.0001554265,"threshold_uncertainty_score":0.008102715},"labels":[],"label_agreement":null},{"id":"W2037567686","doi":"10.1086/508675","title":"Three‐Dimensional Simulations of the Reorganization of a Quark Star’s Magnetic Field as Induced by the Meissner Effect","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Calgary","funders":"","keywords":"Physics; Pulsar; Magnetic field; Astrophysics; Rotation period; Rotation (mathematics); Dipole; Neutron star; Quark star; Magnetar; Stars; Strange matter; Geometry","score_opus":0.005446823666107477,"score_gpt":0.2754871474775205,"score_spread":0.270040323811413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037567686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9732255,0.00026594845,0.0073193563,0.00082967884,0.0001527289,0.00010342338,0.0021417674,0.00032223092,0.015639365],"genre_scores_gemma":[0.9883083,0.00020264692,0.0067925034,0.00024966654,0.000048532165,0.00018724788,0.0015808383,0.00009610909,0.0025340854],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981123,0.000048167112,0.000010454469,0.000025730267,0.000036654757,0.00006772852],"domain_scores_gemma":[0.99860173,0.00078201224,0.0001301343,0.00007606645,0.0001933668,0.00021670928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046549962,0.00071273424,0.0010035636,0.0005461284,0.0009855912,0.0011885936,0.0014689603,0.0021027606,0.0056913123],"category_scores_gemma":[0.0020189427,0.00053405773,0.0011413917,0.0006969539,0.0012285975,0.00062865246,0.0009863267,0.0018629993,0.00028527496],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002671703,0.00021894576,0.003986259,0.00006238585,0.00008198495,0.0002054727,0.00013965275,0.9881563,0.0012934936,0.003341356,0.00093654625,0.001310482],"study_design_scores_gemma":[0.0000854169,0.00004855064,0.0012573039,0.00000841518,0.000011647153,0.000015028687,0.000061862265,0.9969721,0.00025199453,0.00092790165,0.00034846753,0.000011270693],"about_ca_topic_score_codex":0.02552096,"about_ca_topic_score_gemma":0.015698822,"teacher_disagreement_score":0.02552096,"about_ca_system_score_codex":0.0010749947,"about_ca_system_score_gemma":0.0011738804,"threshold_uncertainty_score":0.05074483},"labels":[],"label_agreement":null},{"id":"W2037642463","doi":"10.1088/0004-637x/739/1/20","title":"THE LUMINOSITY PROFILE AND STRUCTURAL PARAMETERS OF THE ANDROMEDA GALAXY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":200,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Bulge; Andromeda Galaxy; Milky Way; Andromeda; Galaxy; Luminosity; Astronomy; Star formation","score_opus":0.010256613195718012,"score_gpt":0.19866416682972346,"score_spread":0.18840755363400544,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037642463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99449015,0.00009811178,0.0030338839,0.000022010669,8.779649e-7,0.0000050965414,0.00047823,0.00007364924,0.0017981193],"genre_scores_gemma":[0.99569076,0.00004193887,0.0030397924,0.0000070424503,0.0000019111305,0.0000044547346,0.00087246543,0.000017994127,0.0003236765],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991786,0.000015529586,0.0000035235319,0.000029025758,0.00001944973,0.0000145385],"domain_scores_gemma":[0.99966776,0.000057297453,0.00006843874,0.00005914802,0.00009616459,0.000051179897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016013806,0.00022217473,0.00009242783,0.00063137553,0.00013080222,0.0003464076,0.00020481522,0.00016340455,0.0010603747],"category_scores_gemma":[0.00064619654,0.00011041369,0.00019981695,0.00040489715,0.00013673522,0.00025894682,0.00022800482,0.00017886877,0.00052084634],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021621825,0.000048967748,0.8275561,0.000051329454,0.00009480269,0.000196512,0.00032705697,0.044834055,0.07676441,0.0023700797,0.00051304867,0.047027465],"study_design_scores_gemma":[0.0000062767863,0.000054825607,0.9543838,0.000008529178,0.00001670026,0.00032086234,0.000094823976,0.03695304,0.0057191798,0.00051787985,0.0019022325,0.000021860533],"about_ca_topic_score_codex":0.004554438,"about_ca_topic_score_gemma":0.004513915,"teacher_disagreement_score":0.004554438,"about_ca_system_score_codex":0.00034314947,"about_ca_system_score_gemma":0.000111378315,"threshold_uncertainty_score":0.009055853},"labels":[],"label_agreement":null},{"id":"W2037665230","doi":"10.1088/0004-637x/752/1/53","title":"DEBRIS DISKS IN<i>KEPLER</i>EXOPLANET SYSTEMS","year":2012,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Exoplanet; Debris; Planetary system; Asteroid; Luminosity; Debris disk; Planet; Asteroid belt; Solar System","score_opus":0.016261033941712424,"score_gpt":0.23205457909517574,"score_spread":0.21579354515346333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037665230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962366,0.00007580983,0.000017535851,0.0000041941757,4.7754554e-7,9.938516e-7,0.00006042882,0.0000027013962,0.00021429682],"genre_scores_gemma":[0.9995577,0.000051823677,0.000059317346,0.0000056912536,0.0000011606951,0.0000018779006,0.0002374704,0.0000015690058,0.00008329026],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999864,0.000010465574,0.000019114534,0.000052325275,0.000018302224,0.00003577767],"domain_scores_gemma":[0.9994867,0.000060998525,0.00026923002,0.000034173507,0.000040394072,0.0001084473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013391365,0.00022877438,0.00018621174,0.0014857767,0.00063680875,0.00075084076,0.00021461253,0.0002886645,0.0009179225],"category_scores_gemma":[0.0005602401,0.00022704987,0.00014099086,0.00085967063,0.0003073613,0.00054299,0.00087892724,0.00015756181,0.00027092695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019850377,0.00002365029,0.98248243,0.00002900276,0.000035805773,0.00026222397,0.0005061636,0.00027313255,0.013593392,0.000081372375,0.00008140226,0.0024329184],"study_design_scores_gemma":[0.000005102279,0.000031811214,0.99763894,0.000004318186,0.000010960999,0.00038387883,0.00026647578,0.00021925762,0.0010421502,0.000057520105,0.00033632905,0.0000032373748],"about_ca_topic_score_codex":0.0021846883,"about_ca_topic_score_gemma":0.002705668,"teacher_disagreement_score":0.0021846883,"about_ca_system_score_codex":0.0004519564,"about_ca_system_score_gemma":0.00010531543,"threshold_uncertainty_score":0.004343927},"labels":[],"label_agreement":null},{"id":"W2037702567","doi":"10.1088/0004-637x/744/2/134","title":"SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC). V. NEW BROWN DWARFS IN ρ OPHIUCHI","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Brown dwarf; Physics; Astrophysics; Subaru Telescope; Photometry (optics); Stars; Astronomy; Very Large Telescope; Population; Spectral line; Spectrograph","score_opus":0.017948240242928026,"score_gpt":0.22584727513357256,"score_spread":0.20789903489064454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037702567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990049,0.00012527865,0.000101597805,0.000006754555,0.0000024446701,0.000006107768,0.00015267776,0.000009829057,0.0005904404],"genre_scores_gemma":[0.99829215,0.00010707025,0.00037493222,0.0000093309145,0.0000054290763,0.0000080801865,0.00085565896,0.000002999113,0.0003442508],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986076,0.000010434287,0.000012020905,0.000030843945,0.00004287133,0.000043029228],"domain_scores_gemma":[0.9995086,0.00004742092,0.00018568078,0.00003476954,0.00006765031,0.00015583175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024183154,0.00015976699,0.00022762903,0.0012965754,0.0006568112,0.0005069934,0.00020485235,0.00010495822,0.0007802972],"category_scores_gemma":[0.00047268026,0.000094758805,0.00014804471,0.0008408333,0.00030267055,0.00022249314,0.00096789934,0.00013371625,0.00013973037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008480478,0.000016160013,0.9802167,0.000032373653,0.000021186117,0.00036194225,0.0005023454,0.00010180145,0.009708489,0.00019625232,0.00023381834,0.008524252],"study_design_scores_gemma":[0.0000025373508,0.000035958958,0.997692,0.0000039555057,0.000008796184,0.00031460734,0.0002320694,0.00013608897,0.0006043838,0.000028844524,0.00093831745,0.0000025066543],"about_ca_topic_score_codex":0.011424272,"about_ca_topic_score_gemma":0.025150066,"teacher_disagreement_score":0.011424272,"about_ca_system_score_codex":0.00036275137,"about_ca_system_score_gemma":0.0002861818,"threshold_uncertainty_score":0.022715569},"labels":[],"label_agreement":null},{"id":"W2037816016","doi":"10.1088/0004-637x/797/2/102","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. XV. THE PHOTOMETRIC REDSHIFT ESTIMATION FOR BACKGROUND SOURCES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; University of British Columbia; St. Mary's University; Herzberg Institute of Astrophysics","funders":"","keywords":"Redshift; Photometric redshift; Virgo Cluster; Galaxy; Magnitude (astronomy); Angular diameter; Redshift survey; Cluster (spacecraft)","score_opus":0.030419879104636387,"score_gpt":0.2508924321666628,"score_spread":0.2204725530620264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037816016","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.039316684,0.0025615322,0.0013158818,0.0016755769,0.0004433611,0.0004618915,0.93562585,0.0011412753,0.017457882],"genre_scores_gemma":[0.06449836,0.001011547,0.0046377475,0.0008395017,0.00016983812,0.00065386074,0.91140103,0.00025286482,0.01653524],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9994686,0.00006729852,0.000046895948,0.000100303005,0.0001909378,0.00012585329],"domain_scores_gemma":[0.9981223,0.0000809854,0.00033775682,0.00024939814,0.00069000066,0.00051948876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015177268,0.0007508461,0.00058841694,0.0062710997,0.0006896976,0.0012135578,0.0017518288,0.00067369884,0.010363015],"category_scores_gemma":[0.0026792523,0.00042231198,0.00056808325,0.006912203,0.00019065439,0.0006556595,0.0019217061,0.00086437346,0.008285472],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026643416,0.00010355478,0.17045815,0.00046644313,0.0002032084,0.00010481284,0.00026536986,0.0005975185,0.0010329921,0.002182878,0.7685169,0.05580172],"study_design_scores_gemma":[0.000102886996,0.000033936623,0.7974824,0.00016216341,0.0000839359,0.00010826804,0.00024754525,0.0003856543,0.00039671792,0.0007555845,0.20021231,0.000028648261],"about_ca_topic_score_codex":0.22998805,"about_ca_topic_score_gemma":0.23482367,"teacher_disagreement_score":0.22998805,"about_ca_system_score_codex":0.0019324318,"about_ca_system_score_gemma":0.0022269005,"threshold_uncertainty_score":0.4572987},"labels":[],"label_agreement":null},{"id":"W2037863202","doi":"10.1088/0004-637x/757/2/187","title":"THE BUILDUP OF A SCALE-FREE PHOTOSPHERIC MAGNETIC NETWORK","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Differential rotation; Dynamo; Photosphere; Astrophysics; Magnetic flux; Statistical physics; Magnetic field; Computational physics","score_opus":0.0038178916810725455,"score_gpt":0.19831519695313812,"score_spread":0.19449730527206557,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037863202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9735839,0.000059948154,0.020349154,0.00028254933,0.000016107522,0.000037108846,0.00014894473,0.00014041949,0.0053818114],"genre_scores_gemma":[0.99609,0.00004026202,0.0032198392,0.00002169735,0.0000045454053,0.000026068747,0.00007943172,0.000025322783,0.00049276056],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.000023838867,0.0000022551776,0.000014652759,0.000013877572,0.000016482021],"domain_scores_gemma":[0.9993918,0.0003137232,0.00007279116,0.00006106526,0.000048164176,0.000112421854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033117126,0.00018859128,0.0002274776,0.0003732085,0.00055826973,0.00072562916,0.0005812617,0.0005859148,0.0015169921],"category_scores_gemma":[0.0021780645,0.00030694666,0.00032959075,0.00024061739,0.0009597258,0.0010217153,0.00048827234,0.0005256111,0.000088664216],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000435775,0.000028657098,0.006339102,0.00001648848,0.00003435305,0.00012975874,0.000074139694,0.98241466,0.0021924183,0.0070826556,0.00023387781,0.0014102861],"study_design_scores_gemma":[0.000020351014,0.000019295387,0.0014931702,0.0000027720976,0.000008030469,0.00002481242,0.000022596576,0.9952087,0.00031289936,0.0026587355,0.0002237714,0.0000049672944],"about_ca_topic_score_codex":0.007980758,"about_ca_topic_score_gemma":0.006512255,"teacher_disagreement_score":0.007980758,"about_ca_system_score_codex":0.0009318544,"about_ca_system_score_gemma":0.0005589001,"threshold_uncertainty_score":0.015868604},"labels":[],"label_agreement":null},{"id":"W2037998204","doi":"10.1088/0004-637x/754/1/37","title":"THE HD 192263 SYSTEM: PLANETARY ORBITAL PERIOD AND STELLAR VARIABILITY DISENTANGLED","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Pennsylvania State University; Pennsylvania Space Grant Consortium; National Aeronautics and Space Administration; National Science Foundation","keywords":"Photometry (optics); Ephemeris; Orbital period; Planet; Light curve; Exoplanet; Radial velocity; Planetary system","score_opus":0.007636252991305423,"score_gpt":0.2050425185499845,"score_spread":0.19740626555867907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2037998204","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99456125,0.0002147066,0.00067216187,0.000035313067,0.0000063021093,0.0000138600335,0.002188941,0.00004553415,0.0022619024],"genre_scores_gemma":[0.9955521,0.000047628,0.0010344133,0.000017087756,0.0000129311775,0.000009701783,0.0028489386,0.000015367787,0.00046181245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998821,0.000015495152,0.000007018318,0.000036384125,0.000032664164,0.00002629718],"domain_scores_gemma":[0.9996655,0.000026880389,0.00013063372,0.0000534918,0.00002490118,0.00009856942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025628434,0.00029643942,0.0002972922,0.0010125629,0.00047931806,0.00037652405,0.00016294136,0.00019811714,0.0019576428],"category_scores_gemma":[0.00042529203,0.00014658495,0.0002060241,0.0014205182,0.00023090332,0.00026704455,0.0003187991,0.0002760813,0.000649393],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012163382,0.00018159718,0.8370821,0.00010592167,0.00012887611,0.0008045748,0.00047020364,0.0009798306,0.12022959,0.0005425522,0.002557736,0.03570069],"study_design_scores_gemma":[0.00001048675,0.00003248872,0.99601775,0.0000032822863,0.000013567589,0.00035343118,0.000029949453,0.0004799397,0.001485939,0.00006718779,0.0015000713,0.000005964473],"about_ca_topic_score_codex":0.011259021,"about_ca_topic_score_gemma":0.024609074,"teacher_disagreement_score":0.011259021,"about_ca_system_score_codex":0.00032230682,"about_ca_system_score_gemma":0.00025759274,"threshold_uncertainty_score":0.022386968},"labels":[],"label_agreement":null},{"id":"W2038077711","doi":"10.1088/0004-637x/781/2/98","title":"THE POLARIZATION SIGNATURE OF LOCAL BULK FLOWS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cosmic microwave background; Polarization (electrochemistry); Quadrupole; Doppler effect; Anisotropy; Intergalactic travel; Microwave","score_opus":0.003086476556671386,"score_gpt":0.2119910537520702,"score_spread":0.20890457719539882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038077711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9840502,0.0002796921,0.005381708,0.00009531629,0.000025826652,0.000006021923,0.0002666586,0.00015979458,0.009734847],"genre_scores_gemma":[0.9981688,0.000120640725,0.00084520085,0.000028541146,0.000053954176,0.0000034382062,0.00014211563,0.000013564874,0.0006237287],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999341,0.000006683785,0.0000010172828,0.000025291258,0.000011131258,0.000021822585],"domain_scores_gemma":[0.9997502,0.00004213536,0.000059279624,0.000031986798,0.000049051963,0.00006738081],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009282327,0.00023985947,0.00017650027,0.0006605415,0.00022643869,0.0004703422,0.00011587724,0.00023667698,0.0020833535],"category_scores_gemma":[0.00031789133,0.00010413764,0.000071627444,0.00042891008,0.00047728143,0.00041377853,0.0003698439,0.00043055892,0.0004261774],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006751019,0.00008177272,0.098103926,0.0001239598,0.00003715958,0.0011087953,0.0003315844,0.0014047794,0.833854,0.010924121,0.002790084,0.05056461],"study_design_scores_gemma":[0.00012395601,0.0004651581,0.683395,0.000054119842,0.00014376297,0.0063919825,0.0007620946,0.015445187,0.2617764,0.021974694,0.009371792,0.00009573628],"about_ca_topic_score_codex":0.00016917927,"about_ca_topic_score_gemma":0.00014142928,"teacher_disagreement_score":0.0020833535,"about_ca_system_score_codex":0.00007506824,"about_ca_system_score_gemma":0.00006016693,"threshold_uncertainty_score":0.0069695115},"labels":[],"label_agreement":null},{"id":"W2038080223","doi":"10.1086/424559","title":"Reaction Rate Uncertainties and the Production of<sup>19</sup>F in Asymptotic Giant Branch Stars","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":215,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Nucleosynthesis; Asymptotic giant branch; Metallicity; Physics; Mixing (physics); Reaction rate; Stellar evolution; Stars; Envelope (radar); Astrophysics; Giant star; Nuclear reaction; Fluorine; Production (economics); Nuclear physics; Chemistry","score_opus":0.01124203176359978,"score_gpt":0.25223690767212775,"score_spread":0.24099487590852797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038080223","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97151226,0.0013977251,0.022064675,0.00014409471,0.00002136976,0.000011728874,0.0010150233,0.00039269394,0.0034403305],"genre_scores_gemma":[0.9967692,0.00021131062,0.0020693536,0.000012512559,0.000010974601,0.000013537601,0.0006432952,0.00008721852,0.00018266824],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99918884,0.00028538983,0.00006121808,0.000159667,0.00021980525,0.00008515792],"domain_scores_gemma":[0.98931736,0.008056999,0.0011565236,0.00073057256,0.00059333845,0.00014520984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025377907,0.0012430139,0.0004827793,0.0009033358,0.0005184601,0.00082224066,0.0014140118,0.0010141883,0.0012759216],"category_scores_gemma":[0.010922951,0.0005587387,0.0014701182,0.000809519,0.00066962483,0.0011038634,0.0007626288,0.00052687165,0.0004376545],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025540777,0.00002653422,0.044899985,0.00007520219,0.00013592289,0.0002340209,0.000064834276,0.94085544,0.0056087994,0.0025497691,0.0001664781,0.0051275566],"study_design_scores_gemma":[0.00006840419,0.00014398611,0.034537252,0.000041977903,0.00018541842,0.0005052053,0.00006671773,0.92344934,0.030090882,0.008779935,0.0020299556,0.00010099318],"about_ca_topic_score_codex":0.0047295135,"about_ca_topic_score_gemma":0.0024440945,"teacher_disagreement_score":0.0047295135,"about_ca_system_score_codex":0.0013734866,"about_ca_system_score_gemma":0.00028274645,"threshold_uncertainty_score":0.0134212375},"labels":[],"label_agreement":null},{"id":"W2038115849","doi":"10.1086/430139","title":"The Fate of Supermassive Black Holes and the Evolution of the <i>M</i> <sub>BH</sub> -σ Relation in Merging Galaxies: The Effect of Gaseous Dissipation","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":143,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Supermassive black hole; Astrophysics; Galaxy; Galaxy merger; Galaxy formation and evolution; Dissipation; Mass ratio; Star formation; Satellite galaxy; Astronomy; Radiative cooling","score_opus":0.002622088683993666,"score_gpt":0.18875766584387804,"score_spread":0.18613557715988438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038115849","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987016,0.00006989634,0.0005367349,0.00006277214,0.0000027136257,0.0000033566182,0.00003222254,0.000012052987,0.000578662],"genre_scores_gemma":[0.99953175,0.00003357764,0.0002855594,0.000017234282,0.0000031540487,0.0000028542268,0.00002783084,0.000007077395,0.00009105934],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999087,0.000021586995,0.000004364647,0.000016993037,0.000011288401,0.000037038975],"domain_scores_gemma":[0.99924755,0.00023563893,0.00023116679,0.000057099503,0.000041785806,0.00018668221],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034570097,0.0003967268,0.00041459818,0.00033910648,0.00062116573,0.0009054409,0.00087134494,0.0008294244,0.0009503921],"category_scores_gemma":[0.0017665976,0.00028823825,0.00046540823,0.0003171415,0.0008414929,0.00088254665,0.00084695587,0.000716156,0.0001533663],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039684848,0.00023562596,0.15606913,0.000053386804,0.00017149709,0.00076160947,0.00057428307,0.808927,0.02105898,0.008037329,0.0003138501,0.00340044],"study_design_scores_gemma":[0.00007981691,0.00017364987,0.039832592,0.000010152044,0.000048110633,0.00010927953,0.00029121482,0.95336956,0.0028722608,0.0028462054,0.0003414404,0.000025788284],"about_ca_topic_score_codex":0.008785871,"about_ca_topic_score_gemma":0.0051742685,"teacher_disagreement_score":0.008785871,"about_ca_system_score_codex":0.000919202,"about_ca_system_score_gemma":0.0003719974,"threshold_uncertainty_score":0.017469466},"labels":[],"label_agreement":null},{"id":"W2038143853","doi":"10.1088/0004-637x/703/1/42","title":"THE COLOR-MAGNITUDE RELATION FOR METAL-POOR GLOBULAR CLUSTERS IN M87: CONFIRMATION FROM DEEP<i>HST</i>/ACS IMAGING","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Astrophysics; Magnitude (astronomy); Physics; Absolute magnitude; Galaxy; Metallicity; Virgo Cluster; Luminosity; Luminosity function; Star cluster; Astronomy; Elliptical galaxy","score_opus":0.005886535544586913,"score_gpt":0.21585177055991903,"score_spread":0.20996523501533212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038143853","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977743,0.00011005523,0.0005732735,0.000039841198,0.0000022387508,0.000003905218,0.00032126266,0.00005549034,0.0011194512],"genre_scores_gemma":[0.998713,0.0000532098,0.00052849116,0.000043825443,0.0000063263114,0.0000033829447,0.0004606321,0.000018947821,0.0001722116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998385,0.000012154403,0.000012233807,0.00004897458,0.00005014511,0.000037876795],"domain_scores_gemma":[0.9983728,0.000213915,0.00056207145,0.0002367245,0.00031756732,0.00029693462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028686857,0.00025511294,0.0002462061,0.0011110044,0.00036713338,0.00086203386,0.00041355987,0.000315298,0.00087895524],"category_scores_gemma":[0.0016152859,0.0001525068,0.00025519053,0.0007915447,0.00054339535,0.00034792232,0.0006798805,0.00040510547,0.0007081757],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004135557,0.00001770564,0.9768074,0.000018528897,0.000023473438,0.00009471496,0.00025148081,0.0002704598,0.017015679,0.00025551073,0.0002866657,0.0049169846],"study_design_scores_gemma":[0.0000018742163,0.000018412193,0.996525,0.000004173123,0.000010857063,0.000108868764,0.000097147975,0.0009317925,0.0018014703,0.00015171035,0.00034544335,0.0000031722961],"about_ca_topic_score_codex":0.0058496227,"about_ca_topic_score_gemma":0.0095494045,"teacher_disagreement_score":0.0058496227,"about_ca_system_score_codex":0.0003363786,"about_ca_system_score_gemma":0.00020627904,"threshold_uncertainty_score":0.011631191},"labels":[],"label_agreement":null},{"id":"W2038159878","doi":"10.1088/0004-637x/739/1/48","title":"DISCOVERY OF TWO L AND T BINARIES WITH WIDE SEPARATIONS AND PECULIAR PHOTOMETRIC PROPERTIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; Brown dwarf; Astrophysics; Proper motion; Luminosity; Spectroscopy; Flux (metallurgy); Effective temperature; Stellar classification; Infrared; Primary (astronomy); Astronomy; Binary number; Stars","score_opus":0.020195006144794816,"score_gpt":0.21806394458400763,"score_spread":0.19786893843921283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038159878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906172,0.0007122525,0.0026733796,0.0006770175,0.00013999332,0.000013942807,0.00039329106,0.00014699186,0.0046259323],"genre_scores_gemma":[0.9970264,0.00007295707,0.0010709483,0.00034469794,0.000075017284,0.0000052215482,0.00034873968,0.000015251867,0.001040835],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99985623,0.000007334491,0.000006661338,0.000060238424,0.000020360165,0.00004914431],"domain_scores_gemma":[0.99937123,0.000092937604,0.00012836757,0.000071793256,0.000053927037,0.00028163687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003255491,0.00027021393,0.0005018847,0.0011290567,0.0016040029,0.0019073617,0.0005452335,0.0015347617,0.0044004805],"category_scores_gemma":[0.00053619844,0.00026602857,0.00034467079,0.0011151152,0.00063777727,0.00061409606,0.0012399649,0.0009499951,0.0011120162],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00419327,0.00066381245,0.4176055,0.00018502933,0.00020205817,0.011135511,0.001168242,0.000615426,0.4776013,0.011535072,0.006789759,0.06830507],"study_design_scores_gemma":[0.00027086586,0.0008844089,0.87486845,0.00003953379,0.00020367093,0.021110678,0.0011026529,0.00449553,0.06284471,0.010287014,0.023754759,0.00013764843],"about_ca_topic_score_codex":0.0005484782,"about_ca_topic_score_gemma":0.0005782326,"teacher_disagreement_score":0.0044004805,"about_ca_system_score_codex":0.00042094823,"about_ca_system_score_gemma":0.00022171257,"threshold_uncertainty_score":0.014721096},"labels":[],"label_agreement":null},{"id":"W2038198163","doi":"10.1086/421698","title":"Evolutionary Properties of Helium‐rich, Degenerate Dwarfs in Binaries Containing Compact Companions","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Physics; Astrophysics; White dwarf; Neutron star; Metallicity; Millisecond pulsar; Brown dwarf; Instability strip; Stellar evolution; Stars; Astronomy; Cepheid variable","score_opus":0.0215639229449548,"score_gpt":0.22653377132984198,"score_spread":0.2049698483848872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038198163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997073,0.00004912532,0.00007867479,0.0000022015872,3.4893085e-7,9.576797e-7,0.00002913245,0.0000020778712,0.00013016262],"genre_scores_gemma":[0.9996543,0.000029766232,0.000095590374,0.0000014788687,0.0000011127693,0.0000010090281,0.000154807,0.0000018166022,0.00006013512],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989593,0.000018128156,0.000010873819,0.000037916743,0.00001792068,0.000019323064],"domain_scores_gemma":[0.9993193,0.00025139799,0.00019632613,0.00004284537,0.00004062891,0.0001494535],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003177329,0.0001590397,0.0003519467,0.0011110404,0.00041923727,0.00080505456,0.00023464915,0.00027354556,0.00048673095],"category_scores_gemma":[0.0014364477,0.00015296819,0.00016081547,0.0006682535,0.00042178432,0.00038082767,0.00048364824,0.00013419347,0.000108675755],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004658691,0.000108850945,0.9396901,0.0000388394,0.00010258761,0.00061250327,0.0002618932,0.02626253,0.02409074,0.0010456544,0.000104179584,0.00721622],"study_design_scores_gemma":[0.000021579137,0.00026482073,0.9341871,0.000013624206,0.00005030533,0.0008352945,0.0003819451,0.058121122,0.0045139296,0.0010821065,0.0005079767,0.000020192536],"about_ca_topic_score_codex":0.0017322659,"about_ca_topic_score_gemma":0.0016373182,"teacher_disagreement_score":0.0017322659,"about_ca_system_score_codex":0.00039654475,"about_ca_system_score_gemma":0.00012698054,"threshold_uncertainty_score":0.0034444332},"labels":[],"label_agreement":null},{"id":"W2038536615","doi":"10.1088/0004-637x/718/2/1085","title":"UNDERSTANDING THE GEOMETRY OF ASTROPHYSICAL MAGNETIC FIELDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Magnetic field; Faraday effect; Rotation (mathematics); L-shell; Line-of-sight; Equipartition theorem; Faraday cage; Field (mathematics); Computational physics; Field strength; Astrophysics; Geometry; Earth's magnetic field; Quantum mechanics","score_opus":0.017886184846318015,"score_gpt":0.2247092828964683,"score_spread":0.20682309805015028,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038536615","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.60026586,0.0131000895,0.26333565,0.002860398,0.0002197498,0.000058860947,0.001827433,0.0011112741,0.11722069],"genre_scores_gemma":[0.9682053,0.0031331277,0.025843523,0.00012620467,0.00014548957,0.00002258618,0.00056093105,0.00007150462,0.0018913314],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99987817,0.000015953876,0.0000044582553,0.000052138374,0.000026463877,0.000022861004],"domain_scores_gemma":[0.9997676,0.000046393845,0.00008013982,0.00002937604,0.000046176847,0.000030376103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011586464,0.00024615118,0.00020828865,0.0006264404,0.00030091256,0.0012246928,0.00054014236,0.00049159507,0.0018601215],"category_scores_gemma":[0.00085452275,0.00028125348,0.000111039604,0.0004835687,0.00082582986,0.0018285704,0.00058506714,0.0007776413,0.0010608875],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017045863,0.00004569396,0.06613267,0.0005918177,0.000050360715,0.00068116444,0.0021195468,0.031033283,0.42277914,0.28751922,0.0068992507,0.18197745],"study_design_scores_gemma":[0.000045599463,0.00014482389,0.37664315,0.0002403394,0.00004025106,0.002554348,0.0022595602,0.0670474,0.043082904,0.37368914,0.13401005,0.00024250615],"about_ca_topic_score_codex":0.0016081019,"about_ca_topic_score_gemma":0.001070048,"teacher_disagreement_score":0.0018601215,"about_ca_system_score_codex":0.0004924174,"about_ca_system_score_gemma":0.00020846388,"threshold_uncertainty_score":0.0062226653},"labels":[],"label_agreement":null},{"id":"W2038634517","doi":"10.1088/0004-637x/763/2/88","title":"COSMOLOGY WITH PHOTOMETRICALLY CLASSIFIED TYPE Ia SUPERNOVAE FROM THE SDSS-II SUPERNOVA SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Los Alamos National Laboratory; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; University of Pittsburgh; University of Cambridge; York University; Science and Technology Facilities Council; Universität Basel; Fermilab; National Science Foundation; Case Western Reserve University; South East Physics Network; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Drexel University; National Aeronautics and Space Administration; U.S. Naval Observatory; U.S. Department of Energy","keywords":"Physics; Cosmic microwave background; Astrophysics; Supernova; Omega; Galaxy; Cosmology; Baryon; Redshift; Type (biology); Dark energy; Cosmological constant; Sky; Mathematical physics","score_opus":0.021624272894128493,"score_gpt":0.24288689670044852,"score_spread":0.22126262380632003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038634517","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98997784,0.00021232046,0.001325795,0.000063027044,0.000009220441,0.000019209976,0.0053906473,0.000056814348,0.0029451773],"genre_scores_gemma":[0.9830888,0.00013721318,0.0013298391,0.000031356827,0.000018010713,0.000017383269,0.014654028,0.000041198124,0.0006821788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99951935,0.00013381091,0.000038348,0.00015857648,0.0000862079,0.000063640946],"domain_scores_gemma":[0.9983968,0.00026166436,0.0004668174,0.00038110447,0.00018289936,0.00031072582],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011445137,0.00033908463,0.00035555693,0.0024913764,0.0004487637,0.0008808144,0.00043179837,0.00014087328,0.0042376495],"category_scores_gemma":[0.0027038197,0.00017375658,0.00042047302,0.0022984957,0.00029622982,0.00037958624,0.00080778485,0.0003659729,0.00094903173],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006126199,0.00004670854,0.9870186,0.000012950914,0.0001336204,0.00007684327,0.00016643209,0.0022425745,0.00051098474,0.0016411868,0.0027291845,0.005359718],"study_design_scores_gemma":[0.000008872728,0.000024718283,0.9834719,0.000012421196,0.00003877785,0.00025226673,0.00020901504,0.009467517,0.00035938664,0.00086125307,0.005275236,0.000018574046],"about_ca_topic_score_codex":0.028040888,"about_ca_topic_score_gemma":0.02911499,"teacher_disagreement_score":0.028040888,"about_ca_system_score_codex":0.00050537876,"about_ca_system_score_gemma":0.00032019388,"threshold_uncertainty_score":0.055755317},"labels":[],"label_agreement":null},{"id":"W2038649309","doi":"10.1088/0004-637x/773/2/86","title":"STAR-FORMING GALAXY EVOLUTION IN NEARBY RICH CLUSTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Star formation; Coma Cluster; Elliptical galaxy; Astronomy; Galaxy; Galaxy cluster; Peculiar galaxy; Luminous infrared galaxy; Galaxy group","score_opus":0.006111146959975783,"score_gpt":0.2031588022959949,"score_spread":0.19704765533601912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038649309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994448,0.000056198816,0.000023297283,0.000011037903,0.0000011026177,0.0000014223677,0.000066635286,0.0000037279171,0.00039174102],"genre_scores_gemma":[0.99965966,0.00002403724,0.00003474827,0.000006825838,0.0000026573287,7.634008e-7,0.00012226598,0.0000013213033,0.00014780802],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998611,0.000020532538,0.0000065878203,0.00005133612,0.000023103215,0.000037315636],"domain_scores_gemma":[0.9995105,0.000032336313,0.00012555227,0.000033549142,0.000041808642,0.00025623044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001595245,0.00015723809,0.00024997312,0.0006889901,0.00076114736,0.0005304291,0.00023245488,0.00024392306,0.0015491061],"category_scores_gemma":[0.00040013378,0.0001263544,0.00016882815,0.000810104,0.00032931307,0.00023841369,0.00050504337,0.00016021672,0.00034789412],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001732142,0.000045999557,0.99078697,0.000013209394,0.00003926911,0.00025306537,0.00030608097,0.00049628475,0.0055074533,0.00023755003,0.00020006465,0.0019409609],"study_design_scores_gemma":[0.0000021974186,0.000022732853,0.9992447,0.0000013520279,0.000005781785,0.00007163665,0.00016177737,0.00025498407,0.00008202763,0.000052134274,0.00009825628,0.0000023892756],"about_ca_topic_score_codex":0.018219978,"about_ca_topic_score_gemma":0.028772172,"teacher_disagreement_score":0.018219978,"about_ca_system_score_codex":0.0005134093,"about_ca_system_score_gemma":0.00020582443,"threshold_uncertainty_score":0.036227822},"labels":[],"label_agreement":null},{"id":"W2038688646","doi":"10.1086/431476","title":"X‐Ray Bursts from the Transient Magnetar Candidate XTE J1810−197","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Flux (metallurgy); RADIUS; Maxima; Black-body radiation; Pulsar; Radiation; Optics","score_opus":0.008666457525641508,"score_gpt":0.2821035210698576,"score_spread":0.2734370635442161,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038688646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917954,0.000049221937,0.000115254836,0.0000123228065,0.0000034309585,0.000003886543,0.00014216622,0.000013750179,0.0004803758],"genre_scores_gemma":[0.9977422,0.000082882005,0.00040348785,0.000028140752,0.00001252899,0.000008946648,0.0012360236,0.0000124273165,0.00047345285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992144,0.00000457437,0.0000063014672,0.000018689372,0.000021249713,0.000027762651],"domain_scores_gemma":[0.99969244,0.000032262138,0.00014656805,0.000032892236,0.000026744694,0.00006913791],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010030858,0.00019607905,0.0002492311,0.00052397593,0.0003813839,0.0005497128,0.00033300277,0.00022479628,0.0010075619],"category_scores_gemma":[0.00026974393,0.00014751838,0.00014278923,0.00056305487,0.00015241317,0.00014440657,0.0003758325,0.00020814927,0.00032778174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008137866,0.00014923862,0.80209714,0.000076798235,0.00010086892,0.0036320277,0.00044858857,0.000535106,0.17617017,0.00024933345,0.0007000666,0.015026877],"study_design_scores_gemma":[0.000022247115,0.00021007805,0.9831572,0.0000120914165,0.000042751682,0.002593962,0.0001675318,0.00071969826,0.010793657,0.000057212877,0.002209957,0.000013658527],"about_ca_topic_score_codex":0.0012243848,"about_ca_topic_score_gemma":0.003576861,"teacher_disagreement_score":0.0012243848,"about_ca_system_score_codex":0.00025225358,"about_ca_system_score_gemma":0.00012045467,"threshold_uncertainty_score":0.0033706427},"labels":[],"label_agreement":null},{"id":"W2038841145","doi":"10.1088/0004-637x/776/2/82","title":"REIONIZATION ON LARGE SCALES. II. DETECTING PATCHY REIONIZATION THROUGH CROSS-CORRELATION OF THE COSMIC MICROWAVE BACKGROUND","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; Cosmic microwave background; Spectral density; Anisotropy; Cosmic background radiation; Redshift; COSMIC cancer database; Polarization (electrochemistry); Cosmic infrared background","score_opus":0.00866566467977212,"score_gpt":0.2511414610280386,"score_spread":0.24247579634826646,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038841145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99440646,0.00011373264,0.0045028254,0.000018641676,0.0000021643507,0.0000040041677,0.00009320403,0.000053407795,0.0008055893],"genre_scores_gemma":[0.9986351,0.000035017358,0.0010657613,0.0000058027163,0.0000041785033,0.000001977199,0.00012242043,0.000016719165,0.000112937414],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998598,0.000018985487,0.0000035518653,0.00005471531,0.000026393725,0.00003652585],"domain_scores_gemma":[0.99885595,0.00028579828,0.00046425665,0.0001864436,0.00006780495,0.00013981064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002951048,0.00027773637,0.00021890644,0.0007633592,0.00015736211,0.0004919218,0.0002691913,0.00018911582,0.0009224956],"category_scores_gemma":[0.0013574893,0.00024120705,0.00028601516,0.0005782452,0.00023680544,0.0005409757,0.00066280825,0.0003327283,0.00013725042],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029742956,0.00005593508,0.8443346,0.000059324535,0.00034068956,0.00038918358,0.00025600195,0.031194786,0.09077847,0.0018833218,0.00042673384,0.029983576],"study_design_scores_gemma":[0.0000069338726,0.00004796305,0.93078625,0.0000049908767,0.00003423289,0.00024119946,0.0000635177,0.06089142,0.006790315,0.00080485974,0.0003141694,0.0000142177105],"about_ca_topic_score_codex":0.0023672725,"about_ca_topic_score_gemma":0.003290922,"teacher_disagreement_score":0.0023672725,"about_ca_system_score_codex":0.0002693664,"about_ca_system_score_gemma":0.00009950109,"threshold_uncertainty_score":0.004706979},"labels":[],"label_agreement":null},{"id":"W2038929406","doi":"10.1086/592373","title":"Kinematic and Chemical Constraints on the Formation of M31’s Inner and Outer Halo","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Metallicity; Halo; Substructure; Galactic halo; Radial velocity; Red giant; Astronomy; Thick disk; Stars; Accretion (finance); Red-giant branch; Star formation; Galaxy","score_opus":0.01436677526148482,"score_gpt":0.20901448192870573,"score_spread":0.1946477066672209,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038929406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99823296,0.0002130652,0.00023570632,0.000017258668,0.0000010319129,0.00000302948,0.00013672776,0.000011854662,0.0011482314],"genre_scores_gemma":[0.9987103,0.00010780942,0.00042573546,0.000017218837,0.0000051051143,0.0000038717103,0.00049130415,0.0000068682143,0.00023179663],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998847,0.000011166039,0.00000717013,0.000025662706,0.00003291501,0.00003841045],"domain_scores_gemma":[0.99952817,0.000046719644,0.00016182296,0.000057905036,0.000067415975,0.00013794142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025947497,0.00028261307,0.00018146723,0.0008547401,0.00044437,0.0005049331,0.00024675857,0.00021732507,0.00091054174],"category_scores_gemma":[0.00061798265,0.00016416886,0.00018679217,0.0005595899,0.00029433463,0.0002466765,0.0007789655,0.00013756423,0.0005634336],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021151495,0.000021006044,0.8737626,0.000034250723,0.00003412767,0.00023377834,0.0005276502,0.0007404717,0.114680305,0.0007160367,0.0002085925,0.008829604],"study_design_scores_gemma":[0.0000037883362,0.000043805485,0.995634,0.0000063663188,0.000007993152,0.00015915948,0.00012629949,0.00064394315,0.002262653,0.00020719784,0.0008997732,0.000005028427],"about_ca_topic_score_codex":0.0034935675,"about_ca_topic_score_gemma":0.0056978324,"teacher_disagreement_score":0.0034935675,"about_ca_system_score_codex":0.00037835806,"about_ca_system_score_gemma":0.0001897648,"threshold_uncertainty_score":0.006946504},"labels":[],"label_agreement":null},{"id":"W2038963855","doi":"10.1086/509648","title":"Density Profiles of Collisionless Equilibria. II. Anisotropic Spherical Systems","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Anisotropy; Halo; Isotropy; RADIUS; Power law; Sigma; Astrophysics; Virial theorem; BETA (programming language); Dark matter; Velocity dispersion; Quantum mechanics; Galaxy; Statistics","score_opus":0.008935813958073722,"score_gpt":0.222907228627868,"score_spread":0.21397141466979427,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038963855","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9066371,0.00038783037,0.04716795,0.000535052,0.00002133362,0.000096863965,0.00067959813,0.00028089853,0.044193376],"genre_scores_gemma":[0.99399066,0.0001358449,0.0031091603,0.00004160425,0.000010319215,0.00002345512,0.00021340098,0.000041150102,0.002434413],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99982566,0.00003201216,0.000010630746,0.000035457928,0.000051080504,0.000045200297],"domain_scores_gemma":[0.9992836,0.00010299349,0.00019163813,0.00008896146,0.00017230488,0.00016057627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035644628,0.00026456607,0.00027318383,0.0010566043,0.00075576134,0.0014130883,0.00091301766,0.00046280646,0.0034279863],"category_scores_gemma":[0.0029130038,0.0003301546,0.00023480025,0.0005843009,0.0010043728,0.0009967487,0.0009285181,0.00054510124,0.0007299825],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003183526,0.00011272784,0.046867777,0.00010847653,0.00007082836,0.00072161475,0.0014546217,0.32243142,0.021007389,0.5868895,0.0041090497,0.01590832],"study_design_scores_gemma":[0.000051636358,0.0000642894,0.026496105,0.000024919353,0.000014542443,0.0003394694,0.0004846115,0.88064235,0.004392233,0.08365544,0.0037521177,0.0000822896],"about_ca_topic_score_codex":0.0074416916,"about_ca_topic_score_gemma":0.0030246323,"teacher_disagreement_score":0.0074416916,"about_ca_system_score_codex":0.0012612693,"about_ca_system_score_gemma":0.00040557398,"threshold_uncertainty_score":0.014796793},"labels":[],"label_agreement":null},{"id":"W2038974650","doi":"10.1086/512660","title":"The Ionization State of Sodium in Galactic Winds","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Photoionization; Ionization; Flux (metallurgy); Luminosity; Galaxy; Infrared; Outflow; Ultraviolet; Absorption (acoustics)","score_opus":0.005524952989232636,"score_gpt":0.21461319486225922,"score_spread":0.20908824187302658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2038974650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987596,0.00016627468,0.000047583824,0.000011614204,0.0000013612407,0.0000010619102,0.000109905144,0.0000029298003,0.0008996425],"genre_scores_gemma":[0.99935836,0.00010808627,0.00005302037,0.000012657472,0.0000019264323,9.909977e-7,0.00023750798,0.0000021048702,0.00022532699],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999076,0.000011131197,0.00000690568,0.000026650761,0.00002069983,0.000026913349],"domain_scores_gemma":[0.9998567,0.000015598753,0.000059195485,0.000007467053,0.000024729074,0.00003635129],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014565214,0.000114056675,0.00015105835,0.00055476377,0.000247946,0.0005452436,0.00022061434,0.00018029254,0.00079610344],"category_scores_gemma":[0.00045084412,0.00011803688,0.00011263347,0.0004818497,0.00020550656,0.00036022704,0.00031110275,0.00009948155,0.000231625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015289898,0.000014262676,0.97647846,0.000017340179,0.00003468699,0.000077305776,0.00019807952,0.00016503588,0.017555702,0.0002827787,0.00013211738,0.004891246],"study_design_scores_gemma":[0.0000033719516,0.000032213597,0.9971105,0.0000061676933,0.000008929676,0.00009435536,0.00021394486,0.0003407214,0.0014012755,0.0001654042,0.00061865064,0.000004399939],"about_ca_topic_score_codex":0.007455187,"about_ca_topic_score_gemma":0.011292923,"teacher_disagreement_score":0.007455187,"about_ca_system_score_codex":0.00037819974,"about_ca_system_score_gemma":0.000087419605,"threshold_uncertainty_score":0.014823616},"labels":[],"label_agreement":null},{"id":"W2039019285","doi":"10.1088/0004-637x/769/1/32","title":"<i>HUBBLE SPACE TELESCOPE</i>IMAGING OF THE BINARY NUCLEUS OF THE PLANETARY NEBULA EGB 6","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec; Université du Québec à Montréal","funders":"","keywords":"White dwarf; Planetary nebula; Nebula; Emission nebula; Protoplanetary nebula; Hubble space telescope; Emission spectrum; Spectroscopy","score_opus":0.006299553588019891,"score_gpt":0.2187409899326,"score_spread":0.2124414363445801,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039019285","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.65779614,0.0042075105,0.015008697,0.002905233,0.0009284691,0.00025059114,0.1327038,0.0041425633,0.18205698],"genre_scores_gemma":[0.8143213,0.0023669908,0.04273241,0.0018175577,0.0005862494,0.00009005653,0.092073776,0.00047396665,0.045537744],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999242,0.0000037774073,0.000003913282,0.000017335355,0.00003273196,0.000018005265],"domain_scores_gemma":[0.9998204,0.000008760084,0.000037693633,0.000020420961,0.00004216823,0.00007056344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018392921,0.000198055,0.00012872744,0.0022506937,0.0003460985,0.0005285857,0.00025325583,0.00030718435,0.010003678],"category_scores_gemma":[0.00020456892,0.000100954574,0.000195782,0.0007550274,0.000103461214,0.0002804443,0.00042662778,0.00039897265,0.00207518],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004473044,0.00013778779,0.19659449,0.0005153811,0.00016685073,0.0026972617,0.00058490486,0.00095647154,0.4871383,0.0032403164,0.2131822,0.09433867],"study_design_scores_gemma":[0.000008416557,0.000029834104,0.9324837,0.000057297737,0.000016431926,0.0012200865,0.0001031493,0.00073571014,0.0064788233,0.00030982486,0.05854141,0.000015280672],"about_ca_topic_score_codex":0.0062598833,"about_ca_topic_score_gemma":0.029072104,"teacher_disagreement_score":0.010003678,"about_ca_system_score_codex":0.00032949803,"about_ca_system_score_gemma":0.00016728036,"threshold_uncertainty_score":0.033465683},"labels":[],"label_agreement":null},{"id":"W2039026120","doi":"10.1086/499428","title":"Rotational Broadening of Atomic Spectral Features from Neutron Stars","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Spectral line; Line (geometry); Redshift; Gravitational redshift; Photosphere; Spectral resolution; Einstein Telescope; Spins","score_opus":0.008529628226711895,"score_gpt":0.2927399365653876,"score_spread":0.2842103083386757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039026120","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99831885,0.00011234068,0.00059279863,0.000017102575,0.0000020474538,0.000001603319,0.000039588653,0.000026417843,0.0008891945],"genre_scores_gemma":[0.9997255,0.00003071005,0.0001020552,0.000005958402,0.0000020857356,8.103862e-7,0.000065389126,0.0000037594546,0.000063611165],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992526,0.000010174142,0.000003962863,0.000017539785,0.000029049179,0.000013992447],"domain_scores_gemma":[0.99962366,0.000097603894,0.00014564492,0.000048378104,0.000040643456,0.000044058892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014761323,0.00015694195,0.0001892966,0.00055471883,0.00017352909,0.00023658719,0.0002101504,0.00019919263,0.0007516336],"category_scores_gemma":[0.00074613915,0.00012449989,0.00015109984,0.00034056747,0.00025835718,0.00020313139,0.00029218596,0.00023104271,0.00018134752],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040014548,0.00008265576,0.5496031,0.00006454338,0.0000671973,0.00045995976,0.00025030915,0.008316009,0.4093181,0.0013155234,0.0004174402,0.029705053],"study_design_scores_gemma":[0.00001095779,0.0000832501,0.960777,0.00000544625,0.000022269334,0.0004774302,0.000068025,0.014722691,0.02222814,0.00066908076,0.0009223044,0.000013434552],"about_ca_topic_score_codex":0.0012001386,"about_ca_topic_score_gemma":0.001229071,"teacher_disagreement_score":0.0012001386,"about_ca_system_score_codex":0.00021895654,"about_ca_system_score_gemma":0.00004485547,"threshold_uncertainty_score":0.0025144815},"labels":[],"label_agreement":null},{"id":"W2039169841","doi":"10.1086/497258","title":"Constrained Cluster Parameters from Sunyaev‐Zel’dovich Observations","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Planck; Cosmic microwave background; Galaxy cluster; Cluster (spacecraft); Line-of-sight; Degeneracy (biology); Astrophysics; Galaxy; Optics","score_opus":0.015007308614196885,"score_gpt":0.21865035100546895,"score_spread":0.20364304239127207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039169841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98003197,0.00037196907,0.007862279,0.00013765469,0.000012344741,0.0000351984,0.0030737137,0.00016313198,0.008311674],"genre_scores_gemma":[0.9932088,0.00017550822,0.0025313527,0.000017953864,0.000010974244,0.000015437618,0.0036493582,0.000032411743,0.00035810162],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981636,0.000025467376,0.000009235679,0.000054323613,0.00004020559,0.00005448258],"domain_scores_gemma":[0.99945384,0.00012975057,0.00012323927,0.00011314142,0.000047774734,0.00013234587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045530655,0.0003836731,0.00038956598,0.0011142142,0.0005186331,0.0011416908,0.00044203468,0.00029704513,0.0019160523],"category_scores_gemma":[0.0019336048,0.00034468787,0.000297093,0.0009354785,0.00034965988,0.0005314299,0.0013114748,0.00040318357,0.00047384144],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082631933,0.000058947102,0.76997906,0.00022325701,0.00032203476,0.000389248,0.0012682639,0.0952547,0.017574154,0.03649038,0.007962821,0.069650784],"study_design_scores_gemma":[0.000114543545,0.00006437939,0.90699,0.00007587273,0.000098254706,0.000112052985,0.00058389717,0.05595308,0.0038627323,0.019967645,0.0120826615,0.00009489647],"about_ca_topic_score_codex":0.024559673,"about_ca_topic_score_gemma":0.029898206,"teacher_disagreement_score":0.024559673,"about_ca_system_score_codex":0.0009143749,"about_ca_system_score_gemma":0.00080850103,"threshold_uncertainty_score":0.04883343},"labels":[],"label_agreement":null},{"id":"W2039233374","doi":"10.1088/0004-637x/693/2/1621","title":"LONG-TERM X-RAY MONITORING OF THE TeV BINARY LS I +61 303 WITH THE<i>ROSSI X-RAY TIMING EXPLORER</i>","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Flux (metallurgy); Orbital period; Binary number; Photon; X-ray; Wavelength; Modulation (music); Astronomy; Optics; Stars","score_opus":0.020628063579610702,"score_gpt":0.24483545967235962,"score_spread":0.22420739609274892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039233374","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99238294,0.00021485036,0.0002924546,0.00007216262,0.000011798437,0.000016458709,0.0050252797,0.00010847645,0.0018754984],"genre_scores_gemma":[0.96398664,0.00023361991,0.0018812184,0.0000999677,0.000050777497,0.000026251351,0.032946568,0.00007974218,0.0006952747],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968207,0.000036943457,0.000021494476,0.00008204367,0.00010017881,0.00007730057],"domain_scores_gemma":[0.999081,0.0000821743,0.00034799852,0.00015640366,0.00012009728,0.000212333],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000483178,0.00036641973,0.00046830284,0.00082822517,0.00037569675,0.0005337241,0.00024968467,0.0003493167,0.00083235814],"category_scores_gemma":[0.0006444099,0.00020929855,0.0003724692,0.00084744906,0.00017996604,0.00028878922,0.00072711334,0.00048371762,0.00085488835],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010832807,0.0004118384,0.8426509,0.00027270682,0.0003889509,0.0017267315,0.0007154062,0.0032829444,0.09008727,0.0005942402,0.012902538,0.04588315],"study_design_scores_gemma":[0.000022489376,0.00013460105,0.9929103,0.000015357704,0.000036274087,0.00045752598,0.00008631853,0.0013820392,0.001544679,0.0000911202,0.003301556,0.00001775954],"about_ca_topic_score_codex":0.005424329,"about_ca_topic_score_gemma":0.017123949,"teacher_disagreement_score":0.005424329,"about_ca_system_score_codex":0.0003210534,"about_ca_system_score_gemma":0.00027017633,"threshold_uncertainty_score":0.01078552},"labels":[],"label_agreement":null},{"id":"W2039250023","doi":"10.1088/0004-637x/705/1/408","title":"THE MASSES OF POPULATION II WHITE DWARFS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of British Columbia","funders":"","keywords":"White dwarf; Massive compact halo object; White (mutation); Population; Astrophysics; Astronomy; Physics; Stars; Biology; Demography; Sociology; Genetics","score_opus":0.008459760861666483,"score_gpt":0.22830022081251336,"score_spread":0.2198404599508469,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039250023","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929261,0.0005707819,0.00017640689,0.000081179176,0.000013047403,0.0000037590353,0.00048104112,0.000012943101,0.0057347976],"genre_scores_gemma":[0.9969494,0.00014596933,0.00009834042,0.000031232663,0.000013193526,0.000003119484,0.00049548957,0.0000058633022,0.002257295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999088,0.000009266858,0.0000043323835,0.000040987274,0.000018742807,0.000017907483],"domain_scores_gemma":[0.9997229,0.000026710766,0.00009431088,0.000016049118,0.00005570475,0.000084362866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019686697,0.00014658467,0.00013264216,0.0007859647,0.00034886244,0.0005916413,0.00019847164,0.00017088224,0.0018047668],"category_scores_gemma":[0.00076196203,0.0000943204,0.00006938626,0.00033874135,0.00022735356,0.00040851795,0.00039934425,0.00016307629,0.00071481435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039380102,0.00003087322,0.93761826,0.00002293874,0.000043029173,0.00015499762,0.001401905,0.00018167275,0.01908078,0.0028368847,0.0023514978,0.03588341],"study_design_scores_gemma":[0.0000046199225,0.000041390707,0.991134,0.0000073573683,0.000009422548,0.00026200278,0.000756674,0.0002068894,0.0008675228,0.0008867219,0.0058186455,0.0000048636516],"about_ca_topic_score_codex":0.0065522175,"about_ca_topic_score_gemma":0.008401831,"teacher_disagreement_score":0.0065522175,"about_ca_system_score_codex":0.00034978424,"about_ca_system_score_gemma":0.0001453382,"threshold_uncertainty_score":0.013028145},"labels":[],"label_agreement":null},{"id":"W2039276693","doi":"10.1088/0004-637x/733/2/100","title":"AN ANALYSIS OF THE PULSATING STAR SDSS J160043.6+074802.9 USING NEW NON-LTE MODEL ATMOSPHERES AND SPECTRA FOR HOT O SUBDWARFS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Blanketing; Physics; Astrophysics; Metallicity; Surface gravity; Spectral line; Effective temperature; Subdwarf; Stars; Line (geometry); Helium; Stellar atmosphere; Dynamo; Astronomy; White dwarf; Magnetic field; Atomic physics","score_opus":0.030203943114933518,"score_gpt":0.25349543507836175,"score_spread":0.22329149196342823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039276693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978834,0.000017717817,0.0010388062,0.00001887927,0.000003464753,0.000006040436,0.0005233877,0.00009300132,0.0004153614],"genre_scores_gemma":[0.99468106,0.00002848716,0.0023541872,0.000014342328,0.0000070154633,0.000016637949,0.0027105457,0.00005363895,0.00013409987],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987376,0.00003298365,0.000009872444,0.000041240146,0.000025069246,0.000017043241],"domain_scores_gemma":[0.9994616,0.00020591356,0.00006839279,0.000117891635,0.00008382777,0.000062365776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000344266,0.00051993167,0.0002617188,0.00042454273,0.00028780382,0.00046382577,0.00059638504,0.0003632469,0.0005584504],"category_scores_gemma":[0.00092928926,0.00022286788,0.0006656938,0.0004211345,0.00025199036,0.00030933678,0.00031881037,0.00026395306,0.0001848443],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007511027,0.00047272033,0.3730908,0.00016406758,0.00043593041,0.00057340675,0.0005113278,0.56562525,0.042208053,0.0015722745,0.0014261081,0.013168925],"study_design_scores_gemma":[0.00018668122,0.00022301092,0.29259396,0.000009170544,0.000080230886,0.00014621955,0.00016345731,0.6961454,0.0077379392,0.0008750478,0.0017997073,0.000039109094],"about_ca_topic_score_codex":0.009007459,"about_ca_topic_score_gemma":0.006792563,"teacher_disagreement_score":0.009007459,"about_ca_system_score_codex":0.00051772577,"about_ca_system_score_gemma":0.00025401614,"threshold_uncertainty_score":0.017910063},"labels":[],"label_agreement":null},{"id":"W2039440221","doi":"10.1088/0004-637x/764/1/61","title":"A WATER MASER AND NH<sub>3</sub>SURVEY OF GLIMPSE EXTENDED GREEN OBJECTS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Maser; Luminosity; Galactic plane; Megamaser; Young stellar object","score_opus":0.010149382477244541,"score_gpt":0.21583949493662888,"score_spread":0.20569011245938434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039440221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992524,0.00002066231,0.00006858615,0.000005198813,4.4086818e-7,0.0000042217466,0.00042760215,0.000006521295,0.00021444676],"genre_scores_gemma":[0.99352056,0.00011040099,0.0009876133,0.000043454715,0.00000785858,0.000022700551,0.004405003,0.000012740938,0.00088968436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998776,0.000012704282,0.00000798544,0.00002919972,0.00002654034,0.00004590573],"domain_scores_gemma":[0.9995315,0.000026602245,0.00013834133,0.000046535522,0.00006712788,0.00018997025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021609318,0.00020083405,0.00017861687,0.0011480023,0.00022527152,0.00023622994,0.00016942254,0.00013154445,0.00072691136],"category_scores_gemma":[0.00032216887,0.00013297572,0.00017170819,0.0005898269,0.0001903409,0.00022942401,0.00065279723,0.0001330932,0.0002835493],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010725153,0.000029854451,0.98274934,0.0000143223,0.000039514944,0.00015175922,0.00037217786,0.00006786782,0.009938713,0.000031247622,0.00033474338,0.006163289],"study_design_scores_gemma":[0.000002066894,0.000022643535,0.9992304,0.0000010634558,0.000007700181,0.000066093344,0.00009580779,0.00004247781,0.00018793152,0.0000061371647,0.00033654846,0.0000012464033],"about_ca_topic_score_codex":0.0065680193,"about_ca_topic_score_gemma":0.020818187,"teacher_disagreement_score":0.0065680193,"about_ca_system_score_codex":0.0001701806,"about_ca_system_score_gemma":0.0001699962,"threshold_uncertainty_score":0.0130595565},"labels":[],"label_agreement":null},{"id":"W2039570859","doi":"10.1088/0004-637x/765/1/41","title":"THE CORRELATION BETWEEN Hα EMISSION AND VISUAL MAGNITUDE DURING LONG-TERM VARIATIONS IN CLASSICAL Be STARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Astrophysics; Physics; Magnitude (astronomy); Stars; Star (game theory); Term (time); Line-of-sight; Rotation (mathematics); Be star; Equivalent width; Astronomy; Emission spectrum; Geometry; Mathematics; Spectral line","score_opus":0.010407074636969882,"score_gpt":0.24439235455961902,"score_spread":0.23398527992264914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039570859","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99945277,0.000026614262,0.00017708888,0.0000052072396,7.728586e-7,0.000001016734,0.00005688814,0.000005490859,0.00027413573],"genre_scores_gemma":[0.99971634,0.0000105696,0.00005844019,0.0000013368841,0.0000012946309,8.603892e-7,0.00013528235,0.0000014139338,0.000074379575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999075,0.000018737455,0.000007903278,0.000032272215,0.000012853759,0.000020751475],"domain_scores_gemma":[0.9982008,0.00063604984,0.0005935079,0.00017623632,0.00015037332,0.00024294994],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035914316,0.00013748278,0.00011312926,0.00063282775,0.00019352125,0.0003711538,0.0002247459,0.0002579346,0.0005511656],"category_scores_gemma":[0.002485878,0.00013080334,0.00016468689,0.00031988966,0.00032138324,0.00044357605,0.00030651822,0.00023888129,0.00019766335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010113111,0.000013821646,0.9934348,0.000005176369,0.000038508417,0.000045225654,0.00005046518,0.0022229524,0.00206305,0.00014365077,0.000046573863,0.0018346111],"study_design_scores_gemma":[0.0000013131797,0.000028553648,0.99449843,0.0000013567716,0.000007608139,0.0000885119,0.0000361349,0.004895234,0.00027655662,0.00010564271,0.000057335154,0.0000032221526],"about_ca_topic_score_codex":0.00223317,"about_ca_topic_score_gemma":0.004431137,"teacher_disagreement_score":0.00223317,"about_ca_system_score_codex":0.00035237076,"about_ca_system_score_gemma":0.000077290286,"threshold_uncertainty_score":0.0044403076},"labels":[],"label_agreement":null},{"id":"W2039769404","doi":"10.1088/0004-637x/695/1/469","title":"SERENDIPITY OBSERVATIONS OF FAR INFRARED CIRRUS EMISSION IN THE SPITZER INFRARED NEARBY GALAXIES SURVEY: ANALYSIS OF FAR-INFRARED CORRELATIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cirrus; Physics; Spitzer Space Telescope; Infrared; Astrophysics; Galaxy; Astronomy; Cosmic infrared background; Cosmic dust; Luminous infrared galaxy; Interstellar medium; Far infrared; Line-of-sight; Photometer; Emissivity; Telescope; Atmospheric sciences","score_opus":0.019527978459785024,"score_gpt":0.24257222935481237,"score_spread":0.22304425089502736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039769404","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99894494,0.000068827634,0.00016277004,0.000010345588,0.0000012913368,0.0000019561594,0.00045275062,0.000008814307,0.00034832064],"genre_scores_gemma":[0.9978131,0.000060882394,0.0002927638,0.00000840566,0.000008847972,0.0000035979426,0.0016249672,0.000005111367,0.00018231157],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974567,0.000045988618,0.000011729764,0.00008388631,0.000057886937,0.00005490093],"domain_scores_gemma":[0.99913496,0.00015766037,0.00031474343,0.00012266805,0.0001100503,0.00015993559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003360382,0.00018021314,0.00017072898,0.0015155546,0.00014379033,0.00031529498,0.00020539176,0.000117867494,0.0006107545],"category_scores_gemma":[0.0007719241,0.00010036043,0.0001966666,0.00086131133,0.00021434975,0.00018313523,0.00036404896,0.0001640737,0.00028459635],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004913038,0.000022902328,0.99138653,0.0000061477576,0.0000598197,0.00005013495,0.000054785698,0.0003760871,0.0033368412,0.00007758242,0.00025538422,0.0043246155],"study_design_scores_gemma":[0.000001072602,0.0000064907217,0.9993911,6.720556e-7,0.000006124539,0.000018507266,0.000015243709,0.00031300393,0.0001188284,0.00001123349,0.00011659674,0.0000010469321],"about_ca_topic_score_codex":0.0044596344,"about_ca_topic_score_gemma":0.007447227,"teacher_disagreement_score":0.0044596344,"about_ca_system_score_codex":0.0001823261,"about_ca_system_score_gemma":0.00010810315,"threshold_uncertainty_score":0.008867323},"labels":[],"label_agreement":null},{"id":"W2039824875","doi":"10.1086/517958","title":"Joint Analysis of Cluster Observations. I. Mass Profile of Abell 478 from Combined X‐Ray, Sunyaev‐Zel’dovich, and Weak‐Lensing Data","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Victoria","funders":"","keywords":"Physics; Dark matter; Astrophysics; Weak gravitational lensing; Cluster (spacecraft); Galaxy cluster; Galaxy; Abell 2744; Gravitational lens; Brightest cluster galaxy; Computer science","score_opus":0.024827432071552274,"score_gpt":0.2361409970488283,"score_spread":0.21131356497727602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039824875","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99468416,0.00011812187,0.0028090244,0.000036570924,0.0000056970584,0.000012241211,0.001132661,0.00014429525,0.0010571718],"genre_scores_gemma":[0.99598914,0.000034112036,0.001960465,0.00000648721,0.0000075634425,0.000009061593,0.0017450728,0.00002781293,0.00022030466],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999495,0.00008307055,0.000035985282,0.0001513275,0.00013965882,0.00009498659],"domain_scores_gemma":[0.99861526,0.00017776112,0.00039854992,0.0003225503,0.00020629089,0.00027950527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007861145,0.00042581154,0.0005056339,0.0018223381,0.0004359444,0.000923456,0.0002900339,0.000223846,0.00062208314],"category_scores_gemma":[0.0018518303,0.0003076621,0.0005284554,0.0012084225,0.00023642193,0.0004300249,0.0012657215,0.00028473017,0.00036253824],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003231419,0.00004620844,0.93066657,0.000057216956,0.00038679558,0.00020048997,0.00027516126,0.009656763,0.03884105,0.00075602235,0.0008668699,0.017923614],"study_design_scores_gemma":[0.000012038158,0.000036606576,0.9519905,0.0000073822343,0.000095401614,0.00009453208,0.00013756253,0.040769022,0.0053857877,0.00034755902,0.001098719,0.000024956564],"about_ca_topic_score_codex":0.015649613,"about_ca_topic_score_gemma":0.025007859,"teacher_disagreement_score":0.015649613,"about_ca_system_score_codex":0.00076280296,"about_ca_system_score_gemma":0.00048964587,"threshold_uncertainty_score":0.031117022},"labels":[],"label_agreement":null},{"id":"W2039943802","doi":"10.1086/318339","title":"The Alignment of the Magnetic Field and Collimated Outflows in Star‐forming Regions: The Case of NGC 2071","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Collimated light; Magnetic field; Field (mathematics); Star formation; Molecular cloud; Magnetohydrodynamics; Star (game theory)","score_opus":0.00980337484178224,"score_gpt":0.23701077816309715,"score_spread":0.22720740332131492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039943802","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982191,0.00012143892,0.000051818533,0.000048152455,0.0000010433206,0.0000018745845,0.00003373517,0.000005165785,0.0015176703],"genre_scores_gemma":[0.99947876,0.00013502815,0.00015587616,0.000009688309,0.000009029376,0.0000020879688,0.000092024486,0.0000035955686,0.000113863745],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998498,0.000026741023,0.000009563217,0.00003165319,0.000029826218,0.000052483458],"domain_scores_gemma":[0.9986833,0.00029359144,0.0006316875,0.00012562517,0.000095324,0.0001703951],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026993017,0.00016289958,0.00022136996,0.001435079,0.0011029479,0.0010820992,0.00037806225,0.0005418964,0.0007193756],"category_scores_gemma":[0.0015364271,0.0001437326,0.00011538337,0.0015277759,0.0010692232,0.0003208848,0.0006129979,0.00027031367,0.00019994691],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026804858,0.000073908624,0.9607804,0.000048852016,0.00003746886,0.011212121,0.0017156572,0.0006893359,0.012454966,0.0026557837,0.0006577937,0.009405753],"study_design_scores_gemma":[0.000013969633,0.00002808316,0.98871976,0.000014933925,0.000032853903,0.005810961,0.0011062426,0.0007459266,0.0014982943,0.00079679134,0.0012168774,0.00001539479],"about_ca_topic_score_codex":0.020678842,"about_ca_topic_score_gemma":0.018241417,"teacher_disagreement_score":0.020678842,"about_ca_system_score_codex":0.0005447405,"about_ca_system_score_gemma":0.00037927282,"threshold_uncertainty_score":0.041116953},"labels":[],"label_agreement":null},{"id":"W2039957573","doi":"10.1088/0004-637x/711/2/655","title":"DENSE GAS TRACERS IN PERSEUS: RELATING THE N<sub>2</sub>H<sup>+</sup>, NH<sub>3</sub>, AND DUST CONTINUUM PROPERTIES OF PRE- AND PROTOSTELLAR CORES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia; National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Millimeter; Nitrogen; Hydrogen; Stars","score_opus":0.008599128789612304,"score_gpt":0.20593001792370771,"score_spread":0.1973308891340954,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2039957573","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99903035,0.00018869425,0.0002015644,0.000009507458,0.0000013761472,0.0000032599244,0.00011584886,0.000017425564,0.00043201135],"genre_scores_gemma":[0.99938226,0.00007469893,0.00026341435,0.000010363184,0.0000022904458,0.0000021079138,0.00015963776,0.0000043913424,0.00010077478],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999602,0.0000042131173,0.0000017475505,0.000015205608,0.000009517705,0.000009095119],"domain_scores_gemma":[0.9998528,0.00003138549,0.000054485867,0.00001032199,0.000021745711,0.000029384706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013550205,0.0003024816,0.00014553471,0.0008204034,0.00016549206,0.00029773184,0.00029360678,0.00015811717,0.00041820845],"category_scores_gemma":[0.0002609633,0.00012371055,0.000096366246,0.00045651017,0.00027189785,0.00023833732,0.00036408938,0.00010343813,0.0001196846],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004343149,0.000047507827,0.92104954,0.000048129303,0.00013046792,0.0005116988,0.0003242644,0.0059948293,0.058131438,0.0003942032,0.00016542451,0.012768214],"study_design_scores_gemma":[0.000029222767,0.00008252071,0.97326136,0.000010947006,0.000033425873,0.00023146992,0.00034119794,0.00942266,0.015329059,0.00046772792,0.00078237563,0.000008050743],"about_ca_topic_score_codex":0.020991392,"about_ca_topic_score_gemma":0.028529631,"teacher_disagreement_score":0.020991392,"about_ca_system_score_codex":0.0005043713,"about_ca_system_score_gemma":0.00013544198,"threshold_uncertainty_score":0.04173839},"labels":[],"label_agreement":null},{"id":"W2040030963","doi":"10.1086/524033","title":"Discovery of Andromeda XIV: A Dwarf Spheroidal Dynamical Rogue in the Local Group?","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Local Group; Andromeda; Andromeda Galaxy; Dwarf galaxy; Galaxy; Dwarf spheroidal galaxy; Satellite galaxy; Halo","score_opus":0.005405899434427499,"score_gpt":0.21110001499767872,"score_spread":0.20569411556325123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040030963","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99460465,0.0023323419,0.0002982879,0.00032247687,0.000021970018,0.0000069782527,0.000101440695,0.000028385584,0.0022836274],"genre_scores_gemma":[0.9983742,0.00047167653,0.0003015717,0.000115186886,0.000032468855,0.0000022421743,0.00011988351,0.000004679385,0.000578054],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998913,0.000012529793,0.0000040060727,0.000046700035,0.00001595573,0.000029427485],"domain_scores_gemma":[0.99972516,0.000019755204,0.00006796959,0.000042706175,0.000015405632,0.00012907774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019833712,0.00018406639,0.00026932862,0.00048044216,0.00062899676,0.00072046235,0.0003035097,0.00042751853,0.0018369429],"category_scores_gemma":[0.0003820784,0.00010859153,0.00013241368,0.00040214753,0.00089349673,0.0005472964,0.0006092187,0.00040405834,0.0006284763],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032031068,0.00006246706,0.9253127,0.000085259555,0.000052462958,0.0036256847,0.0015918082,0.000048088063,0.022753306,0.0018370809,0.0009122922,0.043398574],"study_design_scores_gemma":[0.00001910043,0.00036290984,0.95748574,0.00003873856,0.000047109927,0.019601155,0.002023935,0.000106073276,0.002175366,0.0011439789,0.016972832,0.000023113194],"about_ca_topic_score_codex":0.0024521984,"about_ca_topic_score_gemma":0.0028708212,"teacher_disagreement_score":0.0024521984,"about_ca_system_score_codex":0.00033563894,"about_ca_system_score_gemma":0.00016132937,"threshold_uncertainty_score":0.006145239},"labels":[],"label_agreement":null},{"id":"W2040067310","doi":"10.1088/0004-637x/720/2/1066","title":"A RELATIONSHIP BETWEEN AGN JET POWER AND RADIO POWER","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":472,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Radio galaxy; Astrophysical jet; Scaling; Synchrotron; Relativistic particle; Jet (fluid); Electron; Galaxy cluster; Galaxy","score_opus":0.010322267364653071,"score_gpt":0.2318710472215054,"score_spread":0.2215487798568523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040067310","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905894,0.00036555962,0.0029785645,0.00007882008,0.000006280019,0.0000076790975,0.00032870306,0.000094783376,0.0055502113],"genre_scores_gemma":[0.99876535,0.000055956494,0.0007190519,0.000018996054,0.000011719783,0.0000055811292,0.00020988101,0.000012600788,0.00020094978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973243,0.000037521007,0.000017688983,0.00011506365,0.000062331645,0.000035045407],"domain_scores_gemma":[0.99557096,0.0022540311,0.0010264289,0.0005359509,0.00037962303,0.00023296937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003830434,0.00022732087,0.00018846472,0.0010495016,0.00017727121,0.0008026892,0.00024223216,0.00029723183,0.0020064388],"category_scores_gemma":[0.0054109534,0.00026046543,0.00016197738,0.00086828007,0.0003929111,0.000772927,0.0004771957,0.0005290154,0.0005221228],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007975505,0.000042250955,0.9565571,0.000038820384,0.000062999025,0.00018973561,0.0002310295,0.002719716,0.016053772,0.0017332814,0.00048553693,0.021805951],"study_design_scores_gemma":[0.0000032952987,0.000023952476,0.9953406,0.000004560598,0.0000073533633,0.00028873843,0.00003095241,0.00254952,0.00065200054,0.0007814707,0.00031007171,0.000007482758],"about_ca_topic_score_codex":0.0010267299,"about_ca_topic_score_gemma":0.00068139477,"teacher_disagreement_score":0.0020064388,"about_ca_system_score_codex":0.00022614568,"about_ca_system_score_gemma":0.00009115566,"threshold_uncertainty_score":0.0067121983},"labels":[],"label_agreement":null},{"id":"W2040141814","doi":"10.1086/430127","title":"Multiscale Magnetic Fields in Star‐forming Regions: Interferometric Polarimetry of the MMS 6 Core of OMC‐3","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Magnetic field; Polarimetry; Molecular cloud; Brewster's angle; Stars; Optics; Scattering","score_opus":0.0149367923989889,"score_gpt":0.24759271680940947,"score_spread":0.23265592441042057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040141814","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976388,0.000048033497,0.00027473277,0.00006699023,0.0000088590905,0.000007799026,0.0004928824,0.00006288662,0.00139908],"genre_scores_gemma":[0.9991516,0.000022401411,0.0002718079,0.000017161283,0.000013592132,0.0000032124224,0.0003464751,0.000014449844,0.00015932656],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999442,0.000003954384,0.0000018933086,0.00001745931,0.000014139546,0.000018240054],"domain_scores_gemma":[0.9998568,0.000012816558,0.000035264653,0.000011138702,0.000032801094,0.000051193925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012806007,0.00022272597,0.00037857762,0.00063189893,0.0002823887,0.00039264187,0.000254968,0.00030829487,0.0012348561],"category_scores_gemma":[0.0004113194,0.00021566957,0.0002020537,0.0004795223,0.00020241275,0.00031583954,0.0005545642,0.0002803892,0.00030471844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013924588,0.00024988918,0.57888746,0.0000857193,0.00015333774,0.0006226077,0.0010056644,0.0060718968,0.37440792,0.0009877873,0.0032484392,0.032886796],"study_design_scores_gemma":[0.000022140455,0.000030135665,0.9950925,0.000002994808,0.000014296153,0.00005248536,0.00006052059,0.002582393,0.0016907657,0.00008090922,0.0003637313,0.0000072575926],"about_ca_topic_score_codex":0.007900643,"about_ca_topic_score_gemma":0.011611483,"teacher_disagreement_score":0.007900643,"about_ca_system_score_codex":0.00028212875,"about_ca_system_score_gemma":0.00025428727,"threshold_uncertainty_score":0.01570934},"labels":[],"label_agreement":null},{"id":"W2040160008","doi":"10.1086/308369","title":"Detection of<i>p</i>‐Mode Pulsations and Possible Ellipsoidal Luminosity Variations in the Hot Subdwarf B Star KPD 1930+2752","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Subdwarf; Light curve; Luminosity; Amplitude; Brightness; White dwarf; Stars; Rotation period; Astronomy; Optics; Galaxy","score_opus":0.009591775054866976,"score_gpt":0.22398521684300424,"score_spread":0.21439344178813727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040160008","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991805,0.000023184128,0.00025060528,0.0000073094584,0.0000016169216,0.0000027999408,0.00006386587,0.000012559923,0.00045745113],"genre_scores_gemma":[0.99931943,0.000013832761,0.00042351405,0.0000058939677,0.0000027223984,0.000002328684,0.00014004436,0.000003269066,0.00008882147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999608,0.0000021598735,0.0000022719191,0.000013112176,0.000012677392,0.00000905179],"domain_scores_gemma":[0.9998734,0.000010244316,0.000056281715,0.000008547978,0.00001124378,0.000040318744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000075282085,0.00015688599,0.000108672226,0.00037951712,0.00028586222,0.0002835555,0.00019652057,0.00018720156,0.0004901504],"category_scores_gemma":[0.00024002555,0.00010274938,0.00010362886,0.0003328536,0.00018108093,0.000120352954,0.00021413527,0.00019442271,0.00016113812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046204508,0.000099222685,0.5906749,0.00004111021,0.000050608058,0.0013976112,0.0004260693,0.0010175928,0.38644445,0.00033731997,0.00033537406,0.018713733],"study_design_scores_gemma":[0.000014763604,0.00016700337,0.98109496,0.000003996521,0.000018647537,0.0010861993,0.00012515957,0.0022150327,0.014139397,0.00010028666,0.0010247322,0.000009817513],"about_ca_topic_score_codex":0.0028772193,"about_ca_topic_score_gemma":0.004106053,"teacher_disagreement_score":0.0028772193,"about_ca_system_score_codex":0.00027639023,"about_ca_system_score_gemma":0.00010375711,"threshold_uncertainty_score":0.005720973},"labels":[],"label_agreement":null},{"id":"W2040199079","doi":"10.1088/0004-637x/757/1/48","title":"THE FATE OF DWARF GALAXIES IN CLUSTERS AND THE ORIGIN OF INTRACLUSTER STARS. II. COSMOLOGICAL SIMULATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Intracluster medium; Dwarf galaxy; Galaxy; Galaxy cluster; Galaxy merger; Elliptical galaxy; Galaxy groups and clusters; Cluster (spacecraft)","score_opus":0.011444527241454325,"score_gpt":0.23441195149360047,"score_spread":0.22296742425214616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040199079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.966599,0.00013669577,0.02548877,0.00027340476,0.000024435412,0.00005456098,0.000736496,0.00035112628,0.006335605],"genre_scores_gemma":[0.9742614,0.00012455192,0.022434084,0.000112500114,0.000015878766,0.00008380734,0.0008537863,0.00013043098,0.0019835127],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986434,0.000045438377,0.000006670877,0.000030302797,0.000027052658,0.000026149988],"domain_scores_gemma":[0.9992894,0.00033024396,0.00010600637,0.000085677835,0.000087253946,0.00010141065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005378105,0.00036772204,0.00049119507,0.00049771584,0.00056353165,0.0007667658,0.0016602988,0.0011203699,0.0017673908],"category_scores_gemma":[0.0032584218,0.00043239916,0.00049289386,0.00068413024,0.00059513387,0.00076317915,0.0007413028,0.00063818856,0.00023825781],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046773217,0.000037951613,0.022446686,0.000023275503,0.00003204905,0.000072312905,0.00006260459,0.9692285,0.0011281352,0.0043407422,0.00035779105,0.0022231434],"study_design_scores_gemma":[0.000020438258,0.00000759738,0.0015627246,0.0000026361624,0.000005133316,0.000012173866,0.000015207874,0.99688953,0.00022148195,0.0009855764,0.00027390587,0.0000034850314],"about_ca_topic_score_codex":0.046334222,"about_ca_topic_score_gemma":0.027941491,"teacher_disagreement_score":0.046334222,"about_ca_system_score_codex":0.0016209518,"about_ca_system_score_gemma":0.0011224914,"threshold_uncertainty_score":0.09212905},"labels":[],"label_agreement":null},{"id":"W2040272716","doi":"10.1086/498973","title":"Variable Accretion and Outflow in Young Brown Dwarfs","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Outflow; Accretion (finance); Brown dwarf; Accretion disc; Spectral line","score_opus":0.005639919620984844,"score_gpt":0.21096840808606995,"score_spread":0.2053284884650851,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040272716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99929094,0.00017462777,0.00016196918,0.0000068916215,0.000001919825,0.0000021893666,0.00013323488,0.000008282179,0.00021986861],"genre_scores_gemma":[0.9990409,0.00007514048,0.00023555808,0.00001449713,0.000009137664,0.000002391341,0.00047456397,0.000003848845,0.00014387612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999795,0.000024477624,0.0000126513305,0.0000714045,0.000056644527,0.000039868544],"domain_scores_gemma":[0.99904567,0.00011584301,0.0004553434,0.000060189246,0.00012778961,0.00019517576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043971403,0.00019748964,0.00030705376,0.0010256143,0.00034177562,0.0005970977,0.00024850006,0.00020426644,0.00019011363],"category_scores_gemma":[0.0007633621,0.00010567254,0.0001428802,0.00070409756,0.00023653847,0.00021964761,0.00041680768,0.00019075806,0.00013375196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006841636,0.000022983279,0.9787911,0.000018902392,0.000023728522,0.0002093391,0.000357417,0.00010286657,0.014571361,0.000023308085,0.0000729619,0.0057376255],"study_design_scores_gemma":[8.508892e-7,0.000044548327,0.9986393,0.0000015581221,0.000004999642,0.00026627633,0.00005752652,0.00007283722,0.0006652142,0.000018060087,0.00022694969,0.0000019842987],"about_ca_topic_score_codex":0.0038491732,"about_ca_topic_score_gemma":0.007530879,"teacher_disagreement_score":0.0038491732,"about_ca_system_score_codex":0.00025391564,"about_ca_system_score_gemma":0.00016120358,"threshold_uncertainty_score":0.0076535344},"labels":[],"label_agreement":null},{"id":"W2040277629","doi":"10.1086/513310","title":"The Morphological Content of 10 EDisCS Clusters at 0.5 &lt;<i>z</i>&lt; 0.8","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":153,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Redshift; Context (archaeology); Galaxy; Velocity dispersion; Galaxy cluster; Cluster (spacecraft); Astronomy; Content (measure theory); Star formation; Geography","score_opus":0.01434513133891741,"score_gpt":0.2199534966611461,"score_spread":0.2056083653222287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040277629","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983948,0.000035745208,0.000097829325,0.000008791533,0.0000012668402,0.0000041447074,0.0007234878,0.000027678474,0.0007061468],"genre_scores_gemma":[0.9928911,0.000064869055,0.00066328363,0.000019234378,0.000005808005,0.000011390353,0.005529536,0.000014871937,0.00080005144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998512,0.000006416104,0.000011095268,0.000043829223,0.000036485813,0.000050989434],"domain_scores_gemma":[0.9992606,0.000058978465,0.00022385732,0.000059810198,0.00014650908,0.0002502917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027366346,0.00019370236,0.00020079728,0.0022575324,0.00042522355,0.00049637014,0.00034570936,0.00016467259,0.001468289],"category_scores_gemma":[0.00044678847,0.0001529167,0.00020636599,0.001461016,0.00036933145,0.00022923552,0.0007455215,0.00014900547,0.00033205678],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032214806,0.0000484972,0.9712091,0.00003406787,0.00004005007,0.000187965,0.0006616747,0.0005392619,0.015597343,0.00023869748,0.00083382364,0.010287317],"study_design_scores_gemma":[0.0000020867699,0.000014018552,0.99869627,0.0000017041045,0.0000042771376,0.00005511953,0.000073717645,0.00019620916,0.00058376556,0.000017972217,0.00035241613,0.0000024373883],"about_ca_topic_score_codex":0.00889473,"about_ca_topic_score_gemma":0.01672987,"teacher_disagreement_score":0.00889473,"about_ca_system_score_codex":0.000749133,"about_ca_system_score_gemma":0.00017621474,"threshold_uncertainty_score":0.01768595},"labels":[],"label_agreement":null},{"id":"W2040301200","doi":"10.1086/339280","title":"Do Cooling Flows Survive Cluster Mergers?","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Cooling flow; Astrophysics; Cluster (spacecraft); Turbulence; RADIUS; Accretion (finance); Galaxy cluster; Flow (mathematics); Mechanics; Galaxy","score_opus":0.011213031977637226,"score_gpt":0.21087486963220542,"score_spread":0.19966183765456819,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040301200","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99833006,0.00015721578,0.00043454996,0.00012624719,0.000006805392,0.000008010479,0.00004615484,0.000023269278,0.0008677144],"genre_scores_gemma":[0.99946827,0.0000678768,0.00019074771,0.000024425954,0.000008107577,0.0000033272163,0.0000462797,0.000009020968,0.00018206883],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998017,0.0000471586,0.0000063671455,0.000032591495,0.000020369405,0.000091817754],"domain_scores_gemma":[0.998806,0.00040077078,0.00043025386,0.00008222019,0.000080811194,0.00019987863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007651067,0.00037112192,0.0004984249,0.00039208884,0.0009557847,0.0010610531,0.000599427,0.0008607383,0.0010329295],"category_scores_gemma":[0.0053014676,0.00042747837,0.00030320688,0.0004397289,0.0011198294,0.0011718911,0.0007204373,0.00042198057,0.00015067254],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015915142,0.00031501314,0.43843764,0.00020424474,0.00024732124,0.0026553078,0.0014864841,0.49236798,0.020771293,0.019703038,0.0020379708,0.020182213],"study_design_scores_gemma":[0.00038694104,0.0004980723,0.14703104,0.00003367223,0.00016943584,0.0007728624,0.00091346883,0.8270728,0.0071439724,0.012252642,0.0036536972,0.00007139705],"about_ca_topic_score_codex":0.014239309,"about_ca_topic_score_gemma":0.0092626335,"teacher_disagreement_score":0.014239309,"about_ca_system_score_codex":0.0008618289,"about_ca_system_score_gemma":0.0006113321,"threshold_uncertainty_score":0.028312862},"labels":[],"label_agreement":null},{"id":"W2040377498","doi":"10.1088/0004-637x/716/1/739","title":"IMPLICATIONS OF A HIGH ANGULAR RESOLUTION IMAGE OF THE SUNYAEV-ZEL'DOVICH EFFECT IN RXJ1347–1145","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Bolometer; Angular resolution (graph drawing); Cluster (spacecraft); Telescope; Resolution (logic); Angular diameter; Galaxy cluster; Astronomy; Stars; Optics; Galaxy; Detector","score_opus":0.0033267819043054556,"score_gpt":0.21145557999675324,"score_spread":0.20812879809244778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040377498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978625,0.00010606124,0.00022748492,0.00017993599,0.0000071882473,0.000002197814,0.00012885446,0.00002955552,0.0014562582],"genre_scores_gemma":[0.999539,0.00002751895,0.00014052645,0.000033583296,0.000007726913,0.0000017596421,0.00011590309,0.000008229964,0.00012569048],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998702,0.000015122984,0.0000061232404,0.000028779616,0.000029559256,0.00005027969],"domain_scores_gemma":[0.99967873,0.0000648698,0.000107188804,0.000029398763,0.00002308306,0.00009674175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023259789,0.00013037113,0.0002597886,0.0005909323,0.000382664,0.00066059857,0.00025723517,0.00024027948,0.0016489477],"category_scores_gemma":[0.0004899608,0.0001971089,0.00013563571,0.00027471044,0.00041059952,0.00016765355,0.00082713284,0.00034852416,0.00018741409],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091265806,0.000097509765,0.5275516,0.00009054969,0.00013178508,0.0017926396,0.0008383999,0.0011587486,0.45016637,0.0013488809,0.0011574145,0.0147534795],"study_design_scores_gemma":[0.000011032346,0.000017194516,0.9960402,0.0000043893688,0.000012022576,0.00024320748,0.00010741368,0.00024383893,0.0026463156,0.00006186145,0.000608135,0.000004269792],"about_ca_topic_score_codex":0.004050566,"about_ca_topic_score_gemma":0.006968189,"teacher_disagreement_score":0.004050566,"about_ca_system_score_codex":0.0003851097,"about_ca_system_score_gemma":0.00014757748,"threshold_uncertainty_score":0.008053958},"labels":[],"label_agreement":null},{"id":"W2040431986","doi":"10.1086/368341","title":"Molecular Gas in Candidate Double‐barred Galaxies. II. Cooler, Less Dense Gas Associated with Stronger Central Concentrations","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Star formation; Line (geometry); Peculiar galaxy; Luminous infrared galaxy; Gravitational potential; Galaxy merger; Active galactic nucleus","score_opus":0.007878502993365734,"score_gpt":0.20589978448515903,"score_spread":0.1980212814917933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040431986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99979955,0.0000570373,0.00004028336,0.0000037963287,6.235408e-7,0.0000017895361,0.000017036013,0.0000027907847,0.00007716227],"genre_scores_gemma":[0.99972385,0.000015844633,0.00009251507,0.000008085326,0.0000017641804,0.0000014419941,0.00007629237,0.0000014213043,0.000078816156],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999874,0.000010526117,0.000006643717,0.00003739685,0.00002296661,0.000048348433],"domain_scores_gemma":[0.9994671,0.000036925616,0.00019806872,0.00003054918,0.000052712523,0.00021480562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017890015,0.0002842067,0.00031190133,0.0015044771,0.0003415025,0.0006622179,0.00039591358,0.00033886684,0.0008452527],"category_scores_gemma":[0.00038976283,0.0002232375,0.00017648244,0.00048232672,0.000538608,0.0002489442,0.0006652283,0.0002530152,0.0002148105],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030665912,0.000056061555,0.9318531,0.000017520053,0.000036196547,0.0004920512,0.0003995582,0.00012611144,0.064410456,0.000097455086,0.000034624896,0.0021701623],"study_design_scores_gemma":[0.0000093009885,0.000104763945,0.99625564,0.0000032085563,0.000014586643,0.000575894,0.00033646767,0.0003208003,0.0021253102,0.000040552277,0.0002093588,0.0000040881264],"about_ca_topic_score_codex":0.0028716638,"about_ca_topic_score_gemma":0.0038322757,"teacher_disagreement_score":0.0028716638,"about_ca_system_score_codex":0.00028232596,"about_ca_system_score_gemma":0.00008921865,"threshold_uncertainty_score":0.005709946},"labels":[],"label_agreement":null},{"id":"W2040454561","doi":"10.1086/520926","title":"A Comparative Study of Optical and Ultraviolet Effective Temperatures for DA White Dwarfs from the<i>IUE</i>Archive","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McMaster University","funders":"","keywords":"White dwarf; Balmer series; Stars; Ultraviolet; Extinction (optical mineralogy); Ultraviolet astronomy; Effective temperature; Binary star; Stellar atmosphere; Interstellar medium","score_opus":0.011557632638531481,"score_gpt":0.26427274489582964,"score_spread":0.25271511225729815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040454561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996958,0.00013876718,0.00047712526,0.000008754737,0.000001706442,0.0000025411562,0.0011427833,0.000037966478,0.0012324147],"genre_scores_gemma":[0.99304366,0.000118566,0.001173048,0.0000057643133,0.0000044655576,0.0000048192232,0.0052094692,0.000029692286,0.0004104963],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986136,0.000017093882,0.000010628348,0.000046447294,0.0000428244,0.000021701087],"domain_scores_gemma":[0.99922657,0.00022628068,0.00016508743,0.00009664996,0.00019314229,0.00009235219],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040063038,0.00015404959,0.00022014052,0.0019252552,0.0003902274,0.0005222669,0.00031126416,0.0001717195,0.00076847343],"category_scores_gemma":[0.00090778846,0.00010204711,0.00025413072,0.0015915282,0.00018147174,0.00036736447,0.00026467783,0.0001570418,0.00033045156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027333654,0.00007949693,0.9516436,0.00007682999,0.00013197148,0.00021941519,0.000717868,0.014293853,0.011644022,0.0011326795,0.00097573217,0.018811202],"study_design_scores_gemma":[0.000009488785,0.00006406197,0.97327924,0.0000067711626,0.00003546591,0.00031850807,0.00025396247,0.017721519,0.0042601665,0.00045491057,0.003584686,0.000011243574],"about_ca_topic_score_codex":0.0028542858,"about_ca_topic_score_gemma":0.005522266,"teacher_disagreement_score":0.0028542858,"about_ca_system_score_codex":0.00044377777,"about_ca_system_score_gemma":0.00015056539,"threshold_uncertainty_score":0.0056753755},"labels":[],"label_agreement":null},{"id":"W2040518374","doi":"10.1088/0004-637x/702/2/838","title":"EXPERIMENTAL INVESTIGATIONS OF ION CHARGE DISTRIBUTIONS, EFFECTIVE ELECTRON DENSITIES, AND ELECTRON-ION CLOUD OVERLAP IN ELECTRON BEAM ION TRAP PLASMA USING EXTREME-ULTRAVIOLET SPECTROSCOPY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atomic and Molecular Physics","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF","funders":"","keywords":"Electron beam ion trap; Atomic physics; Ion; Ionization; Electron; Physics; Electron ionization; Cathode ray","score_opus":0.007992278333996137,"score_gpt":0.2528310123668978,"score_spread":0.24483873403290168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040518374","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971871,0.00006337973,0.0020869856,0.000009256682,0.0000010836413,0.000004608378,0.00008766169,0.000032007432,0.0005278853],"genre_scores_gemma":[0.9980552,0.000066018765,0.0015586974,0.0000051950415,0.0000011770352,0.000007062379,0.00010712787,0.000010935152,0.00018863309],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99989474,0.000013171227,0.0000035180276,0.000026064761,0.00003750409,0.000024927445],"domain_scores_gemma":[0.9998442,0.000070093934,0.000023650106,0.0000133499925,0.000035947694,0.000012765968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020960132,0.00026675774,0.00017329447,0.00029504657,0.000265113,0.0002028732,0.00042011958,0.00026011947,0.0008312529],"category_scores_gemma":[0.00038769114,0.00011876941,0.00009331796,0.00040567454,0.0003314132,0.0003214678,0.00026508645,0.0002335116,0.0000949896],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006087598,0.000070022026,0.014357104,0.00007542727,0.000029407605,0.00043935268,0.0003225129,0.0078119696,0.9702139,0.0006251802,0.000116765674,0.0053296303],"study_design_scores_gemma":[0.000038315062,0.000400561,0.037992924,0.000008787078,0.000021590507,0.00039621195,0.0002590348,0.025201477,0.9343335,0.00047431033,0.0008510594,0.000022191833],"about_ca_topic_score_codex":0.00041181175,"about_ca_topic_score_gemma":0.00034306134,"teacher_disagreement_score":0.0008312529,"about_ca_system_score_codex":0.00019182617,"about_ca_system_score_gemma":0.00007266035,"threshold_uncertainty_score":0.002780795},"labels":[],"label_agreement":null},{"id":"W2040538163","doi":"10.1086/587636","title":"Dynamical Blueprints for Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":211,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Queen's University","funders":"","keywords":"Milky Way; Galaxy; Dark matter; Markov chain Monte Carlo; Dark matter halo; Dwarf galaxy problem; Probability distribution; Phase space; Velocity dispersion; Galactic Center","score_opus":0.010563537055431728,"score_gpt":0.21981084598662376,"score_spread":0.20924730893119203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040538163","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.27927428,0.002322702,0.12642486,0.006410899,0.0015846394,0.00029080012,0.0112091815,0.005016219,0.56746644],"genre_scores_gemma":[0.8476947,0.0006576894,0.039672952,0.0006499019,0.000085163825,0.00020132867,0.0036312023,0.0005078935,0.10689907],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997571,0.000067739515,0.000008311226,0.000059819373,0.00006001273,0.000046887522],"domain_scores_gemma":[0.9994653,0.00009016662,0.00005626835,0.00018840662,0.00006663196,0.00013332779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024538703,0.0003029867,0.00023963749,0.0007764542,0.0008775318,0.002196468,0.00081369956,0.000840227,0.04094198],"category_scores_gemma":[0.001617024,0.00015919626,0.00033877802,0.00080532546,0.0008892984,0.0017164029,0.0014882308,0.00089068623,0.0070170495],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008880106,0.00006094628,0.013690316,0.0000734781,0.000014290546,0.0002847795,0.0018700408,0.010394989,0.0014606387,0.87329435,0.037241634,0.061525695],"study_design_scores_gemma":[0.000075262644,0.00009008918,0.012715478,0.00008659514,0.000011464352,0.0006112036,0.001474449,0.030865513,0.0007948369,0.26097813,0.6922428,0.000054195178],"about_ca_topic_score_codex":0.004009463,"about_ca_topic_score_gemma":0.006419027,"teacher_disagreement_score":0.04094198,"about_ca_system_score_codex":0.0011076048,"about_ca_system_score_gemma":0.00052170345,"threshold_uncertainty_score":0.13696456},"labels":[],"label_agreement":null},{"id":"W2040559514","doi":"10.1086/343108","title":"The Jovian Stratosphere after Comet Shoemaker‐Levy/9: Unusual Isotopic Ratios in Molecular Trace Constituents","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Comet; Jovian; Physics; Stratosphere; Jupiter (rocket family); Isotopomers; Astrophysics; Natural abundance; Astrobiology; Astronomy; Radiative transfer; Planet; Isotope; Spectral line; Atmospheric sciences; Nuclear physics; Saturn","score_opus":0.006981075343957948,"score_gpt":0.20419181928752256,"score_spread":0.1972107439435646,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040559514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99558806,0.00023466583,0.00007668862,0.00016304976,0.000032603166,0.00000441435,0.00025189779,0.000020213982,0.0036282537],"genre_scores_gemma":[0.99843174,0.000057415586,0.000050881416,0.00007351322,0.000019778818,0.0000015700718,0.0003358558,0.000012497502,0.0010167853],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991894,0.0000045203633,0.0000028527795,0.000020814661,0.000016552944,0.000036319696],"domain_scores_gemma":[0.9998491,0.000013865961,0.000032875374,0.000014274223,0.000041517884,0.00004839437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019413521,0.0003326937,0.00042656963,0.00065307756,0.0017078285,0.0010574663,0.00038183533,0.0007804032,0.0022333632],"category_scores_gemma":[0.00028575704,0.0001463093,0.00017298738,0.00037384764,0.00058007153,0.000530729,0.00088644703,0.0004876951,0.00068568415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031308986,0.000113240225,0.49336818,0.00007354936,0.00018956511,0.010666196,0.0022441589,0.0003412592,0.4633067,0.0011402899,0.0021911121,0.023234777],"study_design_scores_gemma":[0.000027068132,0.00024233642,0.9809467,0.00000711356,0.000050460043,0.0009341004,0.0010429417,0.00023837172,0.011331849,0.00018691907,0.004982637,0.000009413104],"about_ca_topic_score_codex":0.02500751,"about_ca_topic_score_gemma":0.031755295,"teacher_disagreement_score":0.02500751,"about_ca_system_score_codex":0.00068605476,"about_ca_system_score_gemma":0.0004248014,"threshold_uncertainty_score":0.049723923},"labels":[],"label_agreement":null},{"id":"W2040637318","doi":"10.1088/0004-637x/703/2/1557","title":"DEEP<i>XMM-NEWTON</i>SPECTROSCOPIC AND TIMING OBSERVATIONS OF THE ISOLATED RADIO MILLISECOND PULSAR PSR J0030+0451","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Advanced Research","funders":"","keywords":"Millisecond pulsar; Physics; Astrophysics; Neutron star; Pulsar; RADIUS; Millisecond; Astronomy; Pulsar planet; Binary pulsar","score_opus":0.016161622377561417,"score_gpt":0.2917937740963148,"score_spread":0.2756321517187534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040637318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99482095,0.00027706055,0.0007952174,0.000050499653,0.00000842374,0.0000072970256,0.00045334996,0.000055383844,0.0035318432],"genre_scores_gemma":[0.99627626,0.00009707789,0.0019515433,0.000047328183,0.000013990479,0.000006068508,0.000945052,0.000009516523,0.0006531804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995697,0.0000037142447,0.0000022509691,0.000013085568,0.000013597511,0.000010429441],"domain_scores_gemma":[0.9998054,0.000021420181,0.00009572707,0.000023985758,0.000017241631,0.000036218036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010955485,0.00019496924,0.00014237728,0.0005956633,0.00024216447,0.00028427606,0.0002807798,0.00024691626,0.0014016351],"category_scores_gemma":[0.0003137977,0.00012851613,0.00014016542,0.000369664,0.00018037285,0.00020471039,0.00038242972,0.00019646906,0.00033150168],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072932977,0.00024160564,0.5740351,0.00020934104,0.00017653199,0.0019093204,0.00043226447,0.0030491075,0.33891642,0.0015262592,0.0031760917,0.07559859],"study_design_scores_gemma":[0.000025631465,0.00013748619,0.986485,0.000013681749,0.000038737144,0.0015207448,0.00004879506,0.0017961413,0.006526625,0.0003688139,0.0030257062,0.000012567033],"about_ca_topic_score_codex":0.0013074757,"about_ca_topic_score_gemma":0.003997585,"teacher_disagreement_score":0.0014016351,"about_ca_system_score_codex":0.000197807,"about_ca_system_score_gemma":0.00011538491,"threshold_uncertainty_score":0.0046889186},"labels":[],"label_agreement":null},{"id":"W2040710067","doi":"10.1086/344507","title":"Three‐dimensional Simulations of Jets from Keplerian Disks: Self‐regulatory Stability","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Saint Mary's University","funders":"","keywords":"Physics; Mach number; Jet (fluid); Outflow; Mechanics; Accretion (finance); Hydrostatic equilibrium; Instability; Classical mechanics; Rotational symmetry; Astrophysics; Meteorology","score_opus":0.015190068962759734,"score_gpt":0.2371167780379227,"score_spread":0.22192670907516296,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040710067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9832208,0.00010030183,0.005548018,0.0003149338,0.000036325222,0.000050849216,0.0004161275,0.00015653043,0.010156089],"genre_scores_gemma":[0.9944695,0.000086526576,0.0035201497,0.00009731441,0.000014437623,0.00010103216,0.00040057913,0.000059833892,0.001250576],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998492,0.000032778265,0.000008510322,0.000020754262,0.000038962335,0.00004985659],"domain_scores_gemma":[0.99908805,0.00047559108,0.00009759551,0.000050250994,0.00011095403,0.00017760629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035542843,0.00044933727,0.00069501717,0.00038891606,0.00088925526,0.001324495,0.0012836404,0.0011255167,0.0017962131],"category_scores_gemma":[0.0020552492,0.00038791003,0.0006352942,0.0006406705,0.0010499131,0.0005695473,0.0009290754,0.0011345878,0.00016107359],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013782774,0.00012785454,0.0031629524,0.000020291898,0.000032111668,0.00013116743,0.00011203115,0.99178046,0.0012243069,0.002192397,0.00022631066,0.00085240963],"study_design_scores_gemma":[0.0000535657,0.000021652966,0.0007787515,0.000003486978,0.0000053492317,0.000009253933,0.000031835752,0.997924,0.0003193752,0.00066178857,0.00018230523,0.000008674458],"about_ca_topic_score_codex":0.024944214,"about_ca_topic_score_gemma":0.0115124835,"teacher_disagreement_score":0.024944214,"about_ca_system_score_codex":0.0014417123,"about_ca_system_score_gemma":0.0011649821,"threshold_uncertainty_score":0.04959804},"labels":[],"label_agreement":null},{"id":"W2040730408","doi":"10.1086/425128","title":"Green Bank Telescope Observations of the Eclipse of Pulsar \"A\" in the Double Pulsar Binary PSR J0737-3039","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Research Canada; McGill University; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Pulsar; Eclipse; Physics; Magnetosphere; Astrophysics; Binary pulsar; Green Bank Telescope; Millisecond pulsar; Astronomy; Context (archaeology); Plasma; Geology","score_opus":0.028148774505703602,"score_gpt":0.31089109561535244,"score_spread":0.28274232110964886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040730408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954847,0.00017256063,0.0002653023,0.00005283783,0.000014394122,0.000009401192,0.00070984976,0.000048938866,0.0032421404],"genre_scores_gemma":[0.99634016,0.00016449975,0.0011096986,0.00007596283,0.000022326492,0.000018503188,0.0013169926,0.000023843431,0.0009280442],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987173,0.000011670762,0.000005627231,0.000031648207,0.00003886353,0.000040490722],"domain_scores_gemma":[0.9995815,0.000058465645,0.00011262381,0.00004504916,0.00005978503,0.00014250065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027720517,0.00022948309,0.00030558713,0.0010026122,0.00077731005,0.00044408222,0.0002872145,0.0003314843,0.00089508836],"category_scores_gemma":[0.0003706925,0.00026282753,0.00021697061,0.00064629444,0.00030119816,0.00022354806,0.00055607216,0.00039384075,0.0005528453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009524613,0.00021101563,0.6531863,0.00012277706,0.00014088949,0.0019297443,0.0012350898,0.00100113,0.30870536,0.0010102732,0.006198162,0.025306802],"study_design_scores_gemma":[0.000029875402,0.00011267969,0.9926118,0.000013228902,0.000023413206,0.0005020048,0.00010899772,0.0007163235,0.003544236,0.00008575105,0.002237235,0.000014453539],"about_ca_topic_score_codex":0.013018585,"about_ca_topic_score_gemma":0.031053836,"teacher_disagreement_score":0.013018585,"about_ca_system_score_codex":0.0004953636,"about_ca_system_score_gemma":0.00043808273,"threshold_uncertainty_score":0.025885582},"labels":[],"label_agreement":null},{"id":"W2040797364","doi":"10.1088/0004-637x/696/2/1164","title":"DISCOVERY OF A GIANT Lyα EMITTER NEAR THE REIONIZATION EPOCH","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":155,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Jet Propulsion Laboratory; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; U.S. Department of Energy","keywords":"Physics; Astrophysics; Reionization; Galaxy; Astronomy; Nebula; Star formation; Halo; Subaru Telescope; Stars; Redshift; Spectral line","score_opus":0.005435853069799277,"score_gpt":0.20362354517432704,"score_spread":0.19818769210452777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040797364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99771476,0.00035982847,0.00053435145,0.00007148973,0.000012790393,0.000005135096,0.00011572267,0.000043616736,0.0011422214],"genre_scores_gemma":[0.9972543,0.00023173499,0.0010725776,0.00006349799,0.000030288878,0.000004261718,0.00030405817,0.000006979795,0.0010322605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994373,0.0000024543692,0.0000028790969,0.000019695446,0.000014388006,0.00001688823],"domain_scores_gemma":[0.9997341,0.000027740778,0.0000886315,0.00002579811,0.00003697312,0.00008671329],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015759743,0.00016346875,0.0001695659,0.0005228016,0.000300155,0.0004954821,0.00028190395,0.00040283875,0.001158393],"category_scores_gemma":[0.00022594654,0.00012871996,0.00014950744,0.00021608516,0.00019007974,0.00030975885,0.00047636713,0.00030648345,0.0005430437],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041777862,0.000102801954,0.5787715,0.00010681437,0.00005814695,0.012432888,0.00077884685,0.00021129448,0.36639485,0.0010553265,0.0011238356,0.038545903],"study_design_scores_gemma":[0.000024458568,0.00044258748,0.8898939,0.000025681002,0.00006610266,0.035943843,0.00029257347,0.00076004537,0.05338744,0.0004500327,0.018686714,0.00002656994],"about_ca_topic_score_codex":0.00034116526,"about_ca_topic_score_gemma":0.00043821556,"teacher_disagreement_score":0.001158393,"about_ca_system_score_codex":0.00012261201,"about_ca_system_score_gemma":0.00006195483,"threshold_uncertainty_score":0.003875196},"labels":[],"label_agreement":null},{"id":"W2040940616","doi":"10.1086/508483","title":"Deficit of Wide Binaries in the η Chamaeleontis Young Cluster","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Brown dwarf; Adaptive optics; Stars; Astrophysics; Binary number; Very Large Telescope; Star cluster; Cluster (spacecraft); Astronomy; Exoplanet; Computer science","score_opus":0.006621988363103549,"score_gpt":0.20400122876030233,"score_spread":0.19737924039719879,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040940616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988695,0.00008306283,0.00009275115,0.000012489897,0.0000029726855,0.0000021174133,0.00008985825,0.000008491076,0.00083861966],"genre_scores_gemma":[0.9994173,0.00002320356,0.00006240138,0.0000055956216,0.0000027329331,0.00000121283,0.00013080059,0.0000017526754,0.00035491053],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998797,0.000006435947,0.0000055351534,0.00005208061,0.000027832486,0.000028365765],"domain_scores_gemma":[0.99958664,0.000038034214,0.000120383214,0.000035469096,0.000039688784,0.00017988043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019410819,0.00017331693,0.00027403294,0.0008594082,0.0009828906,0.00072468555,0.00027120864,0.00019800571,0.0031817576],"category_scores_gemma":[0.0006412376,0.00013675896,0.00008282365,0.00038305798,0.00039694033,0.00031609708,0.00075376034,0.00018660721,0.00050056033],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031899984,0.000035114936,0.9702355,0.000020314248,0.000035319,0.00026545976,0.00056841574,0.00027703532,0.019447368,0.0005891196,0.00021141846,0.007996026],"study_design_scores_gemma":[0.0000029445218,0.000042073294,0.9977368,0.000002529967,0.0000077868,0.00023116668,0.0002176586,0.00027607882,0.00061730185,0.00014389194,0.0007172942,0.000004457248],"about_ca_topic_score_codex":0.008877827,"about_ca_topic_score_gemma":0.01958106,"teacher_disagreement_score":0.008877827,"about_ca_system_score_codex":0.00054318254,"about_ca_system_score_gemma":0.00026452847,"threshold_uncertainty_score":0.017652273},"labels":[],"label_agreement":null},{"id":"W2040961169","doi":"10.1086/376748","title":"The Abundance Evolution of Oxygen, Sodium, and Magnesium in Extremely Metal Poor Intermediate-Mass Stars: Implications for the Self-Pollution Scenario in Globular Clusters","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Globular cluster; Isotopes of magnesium; Nucleosynthesis; Magnesium; Stellar evolution; Isotope; Asymptotic giant branch; Abundance (ecology)","score_opus":0.009831348517521162,"score_gpt":0.22483844558480937,"score_spread":0.2150070970672882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040961169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980756,0.000027045626,0.0011658305,0.0000545832,7.931053e-7,0.0000012966075,0.00003544481,0.000016285878,0.0006231202],"genre_scores_gemma":[0.9994854,0.00001998383,0.00025654913,0.0000053872454,9.99712e-7,0.0000013685035,0.000024521905,0.000004138032,0.0002017014],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99997056,0.0000053162066,0.0000018001783,0.000008470284,0.0000056073272,0.000008279399],"domain_scores_gemma":[0.9998516,0.000047414484,0.000038982085,0.000021844937,0.000012708896,0.000027370881],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012612484,0.00025521926,0.00019859694,0.00021221896,0.0003016844,0.0005000762,0.0008300609,0.0005553209,0.0006917765],"category_scores_gemma":[0.0005827511,0.00017364246,0.00038466812,0.00022089998,0.0005070978,0.0005965036,0.0005733228,0.00023202463,0.00011124605],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046389806,0.00010091091,0.2857218,0.000042843963,0.00009480634,0.00056772755,0.0004449062,0.6434329,0.03674701,0.02603501,0.00030612454,0.006041985],"study_design_scores_gemma":[0.00006211353,0.00016608849,0.081995964,0.0000067294454,0.000051492603,0.00030098498,0.00022597643,0.89001983,0.0063698986,0.020207008,0.00055817486,0.000035704776],"about_ca_topic_score_codex":0.006253456,"about_ca_topic_score_gemma":0.0036868036,"teacher_disagreement_score":0.006253456,"about_ca_system_score_codex":0.00070878904,"about_ca_system_score_gemma":0.00019463916,"threshold_uncertainty_score":0.012434125},"labels":[],"label_agreement":null},{"id":"W2040982014","doi":"10.1088/0004-637x/754/2/108","title":"THE CENTRAL BLUE STRAGGLER POPULATION IN FOUR OUTER-HALO GLOBULAR CLUSTERS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Blue straggler; Star cluster; Cluster (spacecraft); Population; Open cluster; Galaxy groups and clusters; Stellar population","score_opus":0.012331865679469168,"score_gpt":0.22723824848970164,"score_spread":0.21490638281023247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2040982014","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9999118,0.000008176999,0.000011182827,0.0000010999709,9.691331e-8,4.870373e-7,0.000028755463,0.0000017256355,0.000036706544],"genre_scores_gemma":[0.9994199,0.000012501238,0.000074860494,0.0000032889463,7.6787853e-7,0.0000013566322,0.0003624344,0.0000024554217,0.00012244351],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998665,0.000016079646,0.0000054509815,0.000051857638,0.000022593389,0.00003737546],"domain_scores_gemma":[0.9995795,0.000053729887,0.00012487201,0.000045814508,0.00006462231,0.00013153539],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002641283,0.00025583417,0.00022180052,0.001207061,0.00032009435,0.00040006777,0.00033421008,0.00022347795,0.00074911513],"category_scores_gemma":[0.0005266972,0.00015038146,0.0001540828,0.000551303,0.00038137988,0.00025942054,0.0006575261,0.00011674867,0.00020836969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021280147,0.000024002895,0.9883532,0.000008776206,0.000033626373,0.0001118849,0.00073798245,0.00038982157,0.0064527863,0.00009490659,0.0000786657,0.0035015787],"study_design_scores_gemma":[0.0000048693023,0.00004129807,0.9987128,0.0000017969214,0.000008773533,0.000077144425,0.00018642987,0.0004920001,0.0003045432,0.000032492662,0.00013424596,0.0000035111088],"about_ca_topic_score_codex":0.018352522,"about_ca_topic_score_gemma":0.031197138,"teacher_disagreement_score":0.018352522,"about_ca_system_score_codex":0.00049490365,"about_ca_system_score_gemma":0.00015560414,"threshold_uncertainty_score":0.036491394},"labels":[],"label_agreement":null},{"id":"W2041049810","doi":"10.1086/524032","title":"Comparison between the Blue and Red Galaxy Alignments Detected in the Sloan Digital Sky Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Galaxy; Astrophysics; Sky; Redshift; Scaling; Weak gravitational lensing; Mathematics; Geometry","score_opus":0.01621481412428088,"score_gpt":0.2530477900953086,"score_spread":0.2368329759710277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041049810","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99727565,0.00010444203,0.00045131973,0.000032755066,0.0000019510978,0.0000015644356,0.0006329678,0.00003758984,0.0014617818],"genre_scores_gemma":[0.99792886,0.00004561693,0.0003946047,0.000016377595,0.000005288178,0.0000023027965,0.0013618354,0.000009080176,0.00023600558],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994481,0.00011442084,0.000029719224,0.00013604604,0.00014145645,0.00013031106],"domain_scores_gemma":[0.9977635,0.00035281669,0.0008517682,0.0002905456,0.0004221135,0.00031922152],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007953335,0.00024258852,0.0002025332,0.0016473485,0.0001870547,0.00060264324,0.00014730277,0.00019245711,0.0006741128],"category_scores_gemma":[0.0020927258,0.00024039864,0.00020003291,0.0012210435,0.0003142929,0.00030564252,0.00061662355,0.000225978,0.00025026142],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001785759,0.000017546903,0.9796498,0.000034197023,0.0001445378,0.000058295445,0.00024470076,0.0010141631,0.011101096,0.0005479574,0.0006374033,0.006371754],"study_design_scores_gemma":[0.0000024984768,0.0000064944015,0.99850637,0.0000018029727,0.000010566638,0.000019227951,0.00002160997,0.0006148498,0.0005186408,0.00003447982,0.00026070615,0.0000027004953],"about_ca_topic_score_codex":0.0062222537,"about_ca_topic_score_gemma":0.01579939,"teacher_disagreement_score":0.0062222537,"about_ca_system_score_codex":0.0004319116,"about_ca_system_score_gemma":0.00021817944,"threshold_uncertainty_score":0.0123720765},"labels":[],"label_agreement":null},{"id":"W2041102574","doi":"10.1088/0004-637x/718/2/666","title":"THE INITIAL CONDITIONS OF CLUSTERED STAR FORMATION. III. THE DEUTERIUM FRACTIONATION OF THE OPHIUCHUS B2 CORE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; National Research Council Canada","funders":"","keywords":"Ophiuchus; Deuterium; Protostar; Fractionation; Line (geometry); Astrochemistry","score_opus":0.017545880809678557,"score_gpt":0.2788972963033995,"score_spread":0.26135141549372093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041102574","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940493,0.00023314498,0.0011282996,0.00005528249,0.000006166234,0.000028284583,0.0004365224,0.000032810756,0.004030198],"genre_scores_gemma":[0.9988078,0.000049239676,0.0003033012,0.000012554566,0.0000025857385,0.000009081744,0.0003184932,0.000004556408,0.00049236364],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993575,0.000004570672,0.0000024759004,0.000015718619,0.000014286137,0.000027187092],"domain_scores_gemma":[0.99987864,0.000014344201,0.000018245593,0.0000112452535,0.000025773925,0.000051821833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009917456,0.00021236288,0.00015737773,0.00023407287,0.00045460963,0.0003901089,0.00023539264,0.00032652324,0.0014337453],"category_scores_gemma":[0.00044761124,0.00014278895,0.00011874516,0.00013353188,0.00025715472,0.00019944596,0.00043942782,0.00026148235,0.00043843072],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010685212,0.00013735628,0.37804475,0.00028641327,0.00009701796,0.002052681,0.0007831004,0.027107706,0.56645006,0.008960643,0.0023829164,0.012628732],"study_design_scores_gemma":[0.00010496219,0.00041937415,0.84908384,0.000044738234,0.000033291686,0.0010391366,0.0012384146,0.023746733,0.110703275,0.0038978404,0.009634693,0.000053658703],"about_ca_topic_score_codex":0.010402151,"about_ca_topic_score_gemma":0.010637867,"teacher_disagreement_score":0.010402151,"about_ca_system_score_codex":0.0008915994,"about_ca_system_score_gemma":0.00036735958,"threshold_uncertainty_score":0.02068317},"labels":[],"label_agreement":null},{"id":"W2041138876","doi":"10.1088/0004-637x/768/1/91","title":"AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: SOURCE CATALOG AND MULTIPLICITY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":326,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; McGill University","keywords":"Galaxy; Submillimeter Array; Star formation; Flux (metallurgy); Multiplicity (mathematics); High resolution; Luminous infrared galaxy; Source counts; Large sample","score_opus":0.010775844272715992,"score_gpt":0.21838365150442915,"score_spread":0.20760780723171315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041138876","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95332414,0.0004599274,0.002070251,0.00015655541,0.000015843732,0.00008996001,0.03774344,0.00064712245,0.0054928246],"genre_scores_gemma":[0.88920087,0.0005098973,0.013513316,0.00017692402,0.000101053716,0.00023709709,0.09196924,0.00016997766,0.004121641],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971515,0.000033962664,0.000019741203,0.000074780284,0.00009374978,0.000062502],"domain_scores_gemma":[0.99827313,0.00017716044,0.00047421988,0.00044110013,0.0002630573,0.0003712208],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006267124,0.00023122695,0.00027001667,0.0050247316,0.0004475899,0.0006252835,0.00057368714,0.00021438308,0.0047631995],"category_scores_gemma":[0.00137362,0.00022629667,0.00027930012,0.003235814,0.00016205337,0.0006582999,0.0008027228,0.00027606287,0.002089469],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002173226,0.00010361244,0.8968724,0.00009355793,0.00008803946,0.000107867265,0.00049377064,0.00045518333,0.012847873,0.0014165828,0.022677844,0.06462591],"study_design_scores_gemma":[0.000012655149,0.000019004405,0.9900746,0.000009367879,0.0000125680235,0.000102619146,0.000044365686,0.00048892794,0.00069741264,0.00015157812,0.00837903,0.000007844044],"about_ca_topic_score_codex":0.01056051,"about_ca_topic_score_gemma":0.02251465,"teacher_disagreement_score":0.01056051,"about_ca_system_score_codex":0.0003991756,"about_ca_system_score_gemma":0.0005695959,"threshold_uncertainty_score":0.02099806},"labels":[],"label_agreement":null},{"id":"W2041460663","doi":"10.1088/0004-637x/690/2/1829","title":"ON THE ENHANCEMENT OF MASS LOSS IN CEPHEIDS DUE TO RADIAL PULSATION. II. THE EFFECT OF METALLICITY","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cepheid variable; Metallicity; Astrophysics; Milky Way; Physics; Large Magellanic Cloud; Astronomy; Luminosity; Galaxy; Stars","score_opus":0.009016523435358113,"score_gpt":0.22154384284220924,"score_spread":0.21252731940685113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041460663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945885,0.0009825759,0.00096981757,0.00012147939,0.0000125935285,0.0000064214432,0.00014019603,0.000030757918,0.0031478105],"genre_scores_gemma":[0.9984957,0.0004248339,0.00023902504,0.00003958513,0.000021295233,0.0000034057396,0.00011240377,0.000009478712,0.0006543387],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998723,0.000024914147,0.000005566005,0.000028039285,0.00002372229,0.00004532967],"domain_scores_gemma":[0.9985424,0.0008045377,0.00031281303,0.00015009005,0.00009020526,0.000099960744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036628457,0.00042787488,0.0001907544,0.00055212434,0.00019247344,0.00039765905,0.00034487655,0.00026006962,0.002353356],"category_scores_gemma":[0.0021780957,0.00009589698,0.0003418185,0.00028940936,0.00031443618,0.00041703045,0.00054188684,0.00035730482,0.00045233956],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003152726,0.00037785457,0.7287233,0.00037903184,0.0002961216,0.0020120519,0.0004990549,0.030406078,0.15410428,0.003906979,0.0012017015,0.07494085],"study_design_scores_gemma":[0.00003748148,0.00096580427,0.9424877,0.000033668686,0.00012373757,0.0013948077,0.00019548714,0.025714602,0.025501607,0.0018851917,0.0016381149,0.00002174278],"about_ca_topic_score_codex":0.0011661041,"about_ca_topic_score_gemma":0.0007363917,"teacher_disagreement_score":0.002353356,"about_ca_system_score_codex":0.000304073,"about_ca_system_score_gemma":0.000077302815,"threshold_uncertainty_score":0.00787282},"labels":[],"label_agreement":null},{"id":"W2041475839","doi":"10.1086/590239","title":"A Multiplicity Census of Young Stars in Chamaeleon I","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Stars; Physics; Multiplicity (mathematics); Brown dwarf; Astrophysics; Telescope; Star formation; Low Mass; Mass ratio; Astronomy","score_opus":0.015683251966785987,"score_gpt":0.22577206830267885,"score_spread":0.21008881633589285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041475839","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988557,0.000087512104,0.00010837822,0.00000798371,8.5097946e-7,0.0000027184428,0.00019578588,0.000008001501,0.0007330811],"genre_scores_gemma":[0.9986539,0.000048117687,0.0002512421,0.000004926579,0.000003373971,0.000002368388,0.0006934365,0.0000031586171,0.000339488],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982196,0.000011410893,0.000008081324,0.00007649759,0.00003689479,0.000045123164],"domain_scores_gemma":[0.9991574,0.00009248152,0.00028013668,0.00007419712,0.00008561263,0.00031011557],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003338146,0.00023541937,0.0002618648,0.0024786734,0.00070785824,0.0006209535,0.00023965418,0.00022875758,0.0015357931],"category_scores_gemma":[0.00086558505,0.00013716669,0.00016144602,0.0009856805,0.0003041368,0.00039012605,0.00069988694,0.00015255435,0.0003364657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014314536,0.000015388841,0.97296023,0.0000133324575,0.000027050455,0.00021600086,0.0006467205,0.00022334639,0.017896103,0.0002939747,0.00014342672,0.0074212817],"study_design_scores_gemma":[0.0000028119869,0.000044758,0.99714583,0.0000018348098,0.000007897974,0.00025843547,0.00014706404,0.00026700785,0.0011363364,0.00008315706,0.000899045,0.0000058866412],"about_ca_topic_score_codex":0.0070141894,"about_ca_topic_score_gemma":0.014883988,"teacher_disagreement_score":0.0070141894,"about_ca_system_score_codex":0.00061139214,"about_ca_system_score_gemma":0.00023441123,"threshold_uncertainty_score":0.013946712},"labels":[],"label_agreement":null},{"id":"W2041675427","doi":"10.1088/0004-637x/791/1/37","title":"THE BLACK HOLE MASS OF NGC 4151. II. STELLAR DYNAMICAL MEASUREMENT FROM NEAR-INFRARED INTEGRAL FIELD SPECTROSCOPY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Reverberation mapping; Stellar kinematics; Black hole (networking); Velocity dispersion; Galaxy; Supermassive black hole; Stellar mass; Bulge; Active galactic nucleus; Mass ratio; Astronomy; Star formation; Milky Way","score_opus":0.007262967924190773,"score_gpt":0.20449288663393908,"score_spread":0.19722991870974832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041675427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99821955,0.00016989143,0.0004371651,0.000018471981,0.0000050799845,0.000004441621,0.00019262626,0.000035194855,0.0009176273],"genre_scores_gemma":[0.9987795,0.000066136075,0.00056479574,0.0000066943207,0.0000060410994,0.0000038027918,0.00038673842,0.0000051763705,0.00018108079],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998461,0.000013879334,0.000009773847,0.000048905415,0.00006125753,0.000019999701],"domain_scores_gemma":[0.9996958,0.000037990005,0.00011153729,0.00005893082,0.000056014662,0.00003971318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026928808,0.00034343536,0.0001503991,0.0010832337,0.00026710308,0.0005094237,0.00038634305,0.00025814938,0.0008468279],"category_scores_gemma":[0.00090694334,0.00011637309,0.00017989261,0.0003079086,0.00035580137,0.00035644099,0.00043600632,0.00020053497,0.00030975853],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022553603,0.000027324091,0.8894729,0.00009798992,0.00007187572,0.00026165356,0.00052858394,0.0033365935,0.07150065,0.00090966374,0.00049576897,0.03307141],"study_design_scores_gemma":[0.00000748668,0.000037400037,0.9879946,0.0000116828305,0.000023147079,0.00015699731,0.00008773487,0.0027501709,0.007864012,0.00022974252,0.0008265267,0.000010343962],"about_ca_topic_score_codex":0.0068027712,"about_ca_topic_score_gemma":0.008287745,"teacher_disagreement_score":0.0068027712,"about_ca_system_score_codex":0.0006699274,"about_ca_system_score_gemma":0.00010637773,"threshold_uncertainty_score":0.01352632},"labels":[],"label_agreement":null},{"id":"W2041768144","doi":"10.1088/0004-637x/799/1/109","title":"EVIDENCE FOR AN ANHYDROUS CARBONACEOUS EXTRASOLAR MINOR PLANET","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planetesimal; White dwarf; Exoplanet; Asteroid; Minor planet; Anhydrous; Helium","score_opus":0.07021801761800349,"score_gpt":0.2836651575078871,"score_spread":0.21344713988988362,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041768144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99811554,0.00008102642,0.000073038515,0.000029413544,0.0000034723707,0.0000028650682,0.000107222855,0.00000841855,0.0015790672],"genre_scores_gemma":[0.99939597,0.00003846849,0.00015880175,0.00002050442,0.0000066293155,0.0000012309577,0.00017144009,0.0000020508517,0.00020474104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999323,0.000004585269,0.000006397249,0.00001855246,0.000022284068,0.000015877238],"domain_scores_gemma":[0.9996569,0.00006376471,0.00010880964,0.000037487698,0.000045690955,0.00008744492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008864638,0.00019052064,0.00013584062,0.00090940075,0.00060882693,0.00040280516,0.00024868207,0.00028285512,0.0024714423],"category_scores_gemma":[0.00041657352,0.00013177683,0.0000916247,0.0005766725,0.00047445204,0.000328304,0.0004720026,0.00018343146,0.0002574383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041110776,0.000071633156,0.7701567,0.000096630596,0.00006551792,0.002184959,0.0006392846,0.00008160955,0.21662298,0.00085409073,0.0002857343,0.008529825],"study_design_scores_gemma":[0.000014307412,0.00021262685,0.9800496,0.0000071237614,0.000028895018,0.004051479,0.0004570587,0.00021069472,0.011764519,0.0002186522,0.0029782916,0.0000067593487],"about_ca_topic_score_codex":0.0016233232,"about_ca_topic_score_gemma":0.0028578844,"teacher_disagreement_score":0.0024714423,"about_ca_system_score_codex":0.00014316796,"about_ca_system_score_gemma":0.0001188895,"threshold_uncertainty_score":0.00826782},"labels":[],"label_agreement":null},{"id":"W2041822254","doi":"10.1086/505560","title":"A Measurement of the CMB 〈EE〉 Spectrum from the 2003 Flight of BOOMERANG","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":260,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Bolometer; Polarization (electrochemistry); Astrophysics; Cosmology; Spectral line; Lambda; Sigma; Spectral density; Planck; Sky; Adiabatic process; Detector; Astronomy; Optics; Quantum mechanics","score_opus":0.006292405549572578,"score_gpt":0.20365590846951512,"score_spread":0.19736350291994254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041822254","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897675,0.00014719248,0.00055188313,0.00015799732,0.000028748598,0.000033915894,0.0038269593,0.00009497408,0.005390818],"genre_scores_gemma":[0.99179614,0.00013667427,0.00200545,0.0001268911,0.000033001066,0.000024425253,0.0049269767,0.000054617045,0.00089580147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998299,0.0000142994,0.0000038142625,0.000040871866,0.00005251756,0.000058554564],"domain_scores_gemma":[0.9996518,0.000023444165,0.000081586615,0.00004488148,0.00007849551,0.00011970357],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002226368,0.0004352012,0.00023262671,0.00096006924,0.00097555027,0.0004921608,0.00029534096,0.00042106683,0.0011638341],"category_scores_gemma":[0.00034283524,0.00021626345,0.00022550426,0.0012186029,0.00042742174,0.0002547136,0.00042353576,0.0006784003,0.0004529786],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009962774,0.00029694007,0.8068618,0.00016623741,0.00036201882,0.00147468,0.002675573,0.0011295566,0.13931592,0.00058216916,0.00887313,0.037265826],"study_design_scores_gemma":[0.000015684967,0.00007124556,0.9886903,0.00000918384,0.000033484663,0.0003115453,0.00013526015,0.00042299586,0.004631757,0.000059433103,0.005596935,0.000022042195],"about_ca_topic_score_codex":0.03473653,"about_ca_topic_score_gemma":0.10671543,"teacher_disagreement_score":0.03473653,"about_ca_system_score_codex":0.00057946536,"about_ca_system_score_gemma":0.0004517921,"threshold_uncertainty_score":0.06906867},"labels":[],"label_agreement":null},{"id":"W2041854675","doi":"10.1086/377070","title":"<i>Chandra</i> Detection of the High Magnetic Field Radio Pulsar J1119-6127in the Supernova Remnant G292.2-0.5","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Pulsar; Supernova remnant; Pulsar wind nebula; Nebula; Luminosity; Magnetic field; Rotational energy; Supernova","score_opus":0.006865400270439899,"score_gpt":0.2519972566805594,"score_spread":0.2451318564101195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041854675","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97867763,0.0013199475,0.0015524375,0.00041357946,0.0001401094,0.000058279096,0.0022884114,0.0003562233,0.015193324],"genre_scores_gemma":[0.9816188,0.00055462646,0.005487041,0.00036495214,0.00013642,0.000037628226,0.006387326,0.00005856908,0.0053545493],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999068,0.000004063037,0.0000058778533,0.000022993483,0.00003205765,0.00002824134],"domain_scores_gemma":[0.9997757,0.000015010189,0.000054397402,0.000042433316,0.000032921373,0.00007964742],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013694947,0.00026232086,0.00020412334,0.0007803481,0.0006802898,0.0005501256,0.00042657452,0.00043678193,0.0029137752],"category_scores_gemma":[0.0002302451,0.00015264297,0.00020334551,0.0004475771,0.000372226,0.00023184993,0.000645401,0.00051504443,0.0009136177],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007023852,0.0003419051,0.13542345,0.00045433897,0.00018324752,0.012065714,0.000338673,0.00041935412,0.7917616,0.0024166068,0.01655084,0.039341874],"study_design_scores_gemma":[0.00009771393,0.0006737996,0.74952185,0.00004769487,0.00015213821,0.031095963,0.00023919636,0.00092614494,0.14480197,0.0010284251,0.07133268,0.00008244739],"about_ca_topic_score_codex":0.0013817666,"about_ca_topic_score_gemma":0.00400203,"teacher_disagreement_score":0.0029137752,"about_ca_system_score_codex":0.0002166556,"about_ca_system_score_gemma":0.00024202968,"threshold_uncertainty_score":0.009747565},"labels":[],"label_agreement":null},{"id":"W2041920307","doi":"10.1086/341351","title":"Completeness in Weak‐Lensing Searches for Clusters","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Completeness (order theory); Weak gravitational lensing; Line-of-sight; Gravitational lens; Physics; Astrophysics; Galaxy; Strong gravitational lensing; Gravitational lensing formalism; Sky; Galaxy cluster; Computer science; Mathematics; Mathematical analysis","score_opus":0.029133256160187526,"score_gpt":0.237893172586016,"score_spread":0.20875991642582847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2041920307","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994806,0.00016703548,0.00380812,0.00008992131,0.0000021160172,0.000012056836,0.00024316732,0.00008299541,0.0007886372],"genre_scores_gemma":[0.99660385,0.0000685668,0.002566675,0.000010737708,0.0000033050712,0.000010076163,0.0005632642,0.000021693044,0.00015187815],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9970982,0.0013798462,0.0001907413,0.0004297505,0.00062056194,0.0002808607],"domain_scores_gemma":[0.9482444,0.03427652,0.0063018426,0.0057629193,0.0036892584,0.0017250457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010583418,0.0004315305,0.0010054422,0.0016395687,0.0009966528,0.002476115,0.0012065736,0.00095425517,0.00068203994],"category_scores_gemma":[0.071269706,0.0007598831,0.00055672554,0.001458318,0.0018171662,0.0024470272,0.0017842513,0.00051424024,0.00022879902],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016054176,0.00012909566,0.4010229,0.00018148338,0.00043914624,0.00015671217,0.00091846014,0.5554041,0.0034670786,0.012823063,0.0009737039,0.02287883],"study_design_scores_gemma":[0.00013600543,0.0002866979,0.15268902,0.00004542271,0.00012410863,0.00025093477,0.0003493996,0.8172301,0.005598215,0.02217386,0.0010310465,0.0000852595],"about_ca_topic_score_codex":0.01100653,"about_ca_topic_score_gemma":0.0073924917,"teacher_disagreement_score":0.01100653,"about_ca_system_score_codex":0.0015984494,"about_ca_system_score_gemma":0.0016298944,"threshold_uncertainty_score":0.055971146},"labels":[],"label_agreement":null},{"id":"W2042049408","doi":"10.1088/0004-637x/803/2/78","title":"MERGERS IN GALAXY GROUPS. II. THE FUNDAMENTAL PLANE OF ELLIPTICAL GALAXIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"University of Toronto; Government of Ontario; Canada Research Chairs; National Science Council; National Research Council Canada; Compute Canada","keywords":"Fundamental plane (elliptical galaxies); Physics; Astrophysics; Elliptical galaxy; Virial theorem; Dark matter; Velocity dispersion; Galaxy; Lenticular galaxy","score_opus":0.012576902896137604,"score_gpt":0.2200955930221589,"score_spread":0.20751869012602128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042049408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99544466,0.00034642685,0.0022741263,0.000085755564,0.000006574264,0.000018090808,0.00018656113,0.00002350848,0.0016142842],"genre_scores_gemma":[0.9986331,0.0000866045,0.0008829629,0.000012808223,0.00000498761,0.000010086671,0.00019578236,0.000008374451,0.0001652834],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9997826,0.000057900506,0.000011552545,0.000061249906,0.000038530343,0.000048205067],"domain_scores_gemma":[0.999183,0.00018840533,0.00034780774,0.000114203234,0.000052741987,0.00011379987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005515135,0.00032252198,0.00026868464,0.00045143606,0.000533437,0.0009450629,0.00043486134,0.00041297462,0.0012444438],"category_scores_gemma":[0.0027858405,0.0002530671,0.00044901145,0.00046944633,0.0010658391,0.0010695558,0.0010197136,0.0003906789,0.00021997163],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044194114,0.00012417753,0.44455472,0.000098398275,0.00022918292,0.00018325761,0.0008138319,0.4982096,0.012523314,0.028179424,0.0011924233,0.013449759],"study_design_scores_gemma":[0.00017978632,0.00040845113,0.35059112,0.00004409153,0.00010723641,0.00043736704,0.00083478016,0.59448266,0.0040972866,0.041772928,0.0069866325,0.00005757473],"about_ca_topic_score_codex":0.006363845,"about_ca_topic_score_gemma":0.0038972232,"teacher_disagreement_score":0.006363845,"about_ca_system_score_codex":0.0007757384,"about_ca_system_score_gemma":0.0002679259,"threshold_uncertainty_score":0.012653589},"labels":[],"label_agreement":null},{"id":"W2042149220","doi":"10.1088/0004-637x/787/2/167","title":"HIGH-ENERGY EMISSION OF THE FIRST MILLISECOND PULSAR","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Millisecond pulsar; Pulsar; Fermi Gamma-ray Space Telescope; Millisecond; Spectral index; Pulse (music); Photon; X-ray pulsar","score_opus":0.006341338012913207,"score_gpt":0.2563748895145601,"score_spread":0.2500335515016469,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042149220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99688333,0.0008521127,0.0004279916,0.000033365777,0.0000099001945,0.000005897717,0.00014318092,0.000035675403,0.0016085404],"genre_scores_gemma":[0.99801576,0.0003915586,0.00080717047,0.000027760765,0.00003301999,0.000006221343,0.00030568207,0.000010220819,0.00040245813],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994636,0.0000037245484,0.000002899,0.000013115863,0.000016079075,0.00001786689],"domain_scores_gemma":[0.9998323,0.000024537856,0.000066478344,0.000018569262,0.000024689258,0.000033441796],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000113127644,0.00021946675,0.00025090482,0.0009617108,0.00033226926,0.0004094447,0.0002825931,0.000250573,0.0009049458],"category_scores_gemma":[0.00025479353,0.00013609148,0.00014061976,0.00073351833,0.0002021568,0.00022419372,0.00037666643,0.00021773286,0.00023569247],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005313953,0.00022762538,0.4636684,0.00026913194,0.0001717643,0.0030962233,0.0007958526,0.000919221,0.4535855,0.002127364,0.001453485,0.07315409],"study_design_scores_gemma":[0.000023814084,0.00027404496,0.9546698,0.000026001479,0.000064905355,0.0028141842,0.00012892153,0.0008773981,0.03376074,0.0008785013,0.00646183,0.00001975091],"about_ca_topic_score_codex":0.0010765987,"about_ca_topic_score_gemma":0.001825591,"teacher_disagreement_score":0.0010765987,"about_ca_system_score_codex":0.00021663203,"about_ca_system_score_gemma":0.000093303366,"threshold_uncertainty_score":0.0030273795},"labels":[],"label_agreement":null},{"id":"W2042172896","doi":"10.1086/501420","title":"Dielectronic Recombination of Fe<scp>xxiii</scp>Forming Fe<scp>xxii</scp>: Laboratory Measurements and Theoretical Calculations","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atomic and Molecular Physics","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Atomic physics; Beryllium; Resonance (particle physics); Ion; Ionization; Nuclear physics; Quantum mechanics","score_opus":0.006945058323088322,"score_gpt":0.22334197933172734,"score_spread":0.21639692100863903,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042172896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925251,0.00017917302,0.005734354,0.00003764822,0.0000037385441,0.000015342508,0.00008627121,0.000106927575,0.0013113385],"genre_scores_gemma":[0.9968569,0.00005861219,0.0028329694,0.0000066581356,0.0000013604537,0.000008750686,0.00006888858,0.000010241247,0.00015567393],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9997508,0.000053894142,0.0000122339,0.00005937284,0.00007477417,0.00004891507],"domain_scores_gemma":[0.999564,0.000190993,0.00008291576,0.00007295223,0.000055058565,0.000034073764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009046471,0.00045282536,0.00029412366,0.0003683418,0.000373288,0.00035078454,0.00072466384,0.00037995513,0.000694642],"category_scores_gemma":[0.0012463406,0.0002273579,0.00021282179,0.0002866646,0.0004000453,0.00039309377,0.00027711503,0.00039703766,0.00018333197],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001132784,0.00035008695,0.04460567,0.00042380908,0.00014694018,0.00079978764,0.0006526562,0.07946527,0.8392818,0.010203366,0.00074528996,0.022192543],"study_design_scores_gemma":[0.00010438118,0.00055085676,0.017567787,0.000013605363,0.000035065495,0.0004328233,0.00010454376,0.16159108,0.81724036,0.0008796304,0.0014319551,0.000047909652],"about_ca_topic_score_codex":0.0016749782,"about_ca_topic_score_gemma":0.0011924267,"teacher_disagreement_score":0.0016749782,"about_ca_system_score_codex":0.001296347,"about_ca_system_score_gemma":0.0002568112,"threshold_uncertainty_score":0.009405673},"labels":[],"label_agreement":null},{"id":"W2042273091","doi":"10.1088/0004-637x/794/1/35","title":"PRECISE ATMOSPHERIC PARAMETERS FOR THE SHORTEST-PERIOD BINARY WHITE DWARFS: GRAVITATIONAL WAVES, METALS, AND PULSATIONS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Astrophysics; Instability strip; Gravitational wave; Low Mass; Effective temperature; Binary number; Surface gravity; Gravitation; Atmosphere (unit); Astronomy; Stars; Thermodynamics","score_opus":0.014225759494565077,"score_gpt":0.29267961330652265,"score_spread":0.2784538538119576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042273091","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9845405,0.00045431693,0.008991162,0.00005697702,0.00001082395,0.000009639984,0.003037663,0.000236215,0.0026626333],"genre_scores_gemma":[0.9900377,0.00013295807,0.006358304,0.000010177448,0.000010309286,0.0000064849987,0.0030297672,0.00003463698,0.00037973814],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993646,0.000008197979,0.000008799141,0.00001898294,0.000021855358,0.0000057762118],"domain_scores_gemma":[0.999726,0.000047871763,0.00008169273,0.000057135618,0.00006456401,0.000022746559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020113913,0.00022229445,0.00018561151,0.000996488,0.00036215413,0.00036204397,0.00023133168,0.00013390204,0.00077885046],"category_scores_gemma":[0.0007296765,0.00010190932,0.00016289958,0.00089120993,0.00009245155,0.0003343449,0.0002876664,0.00020078331,0.00040778317],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000790399,0.00002203985,0.9487757,0.00004206273,0.000041067193,0.00005642449,0.00021067982,0.005279211,0.0152135985,0.000726723,0.00072454725,0.028828882],"study_design_scores_gemma":[0.00001643274,0.00004452447,0.9642994,0.000011856846,0.00005104376,0.00025157153,0.000100352845,0.016694896,0.009979341,0.0015742608,0.0069623785,0.000013978936],"about_ca_topic_score_codex":0.00633374,"about_ca_topic_score_gemma":0.009469996,"teacher_disagreement_score":0.00633374,"about_ca_system_score_codex":0.00032160085,"about_ca_system_score_gemma":0.00020438468,"threshold_uncertainty_score":0.012593746},"labels":[],"label_agreement":null},{"id":"W2042379572","doi":"10.1088/0004-637x/779/1/60","title":"OBLIQUE SHOCK BREAKOUT IN SUPERNOVAE AND GAMMA-RAY BURSTS. I. DYNAMICS AND OBSERVATIONAL IMPLICATIONS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Supernova; Shock (circulatory); Astrophysics; Ejecta; Oblique shock; Jet (fluid); Mechanics; Shock wave","score_opus":0.014261320212147611,"score_gpt":0.23559072361600486,"score_spread":0.22132940340385726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042379572","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889529,0.003340104,0.0036217691,0.00031579554,0.00002178289,0.000013282549,0.00014124249,0.00004065619,0.003552492],"genre_scores_gemma":[0.99687165,0.0020354548,0.00045966357,0.0000408537,0.00004776678,0.0000051409643,0.00018456235,0.000009598817,0.0003453568],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998729,0.00003463283,0.000017675482,0.000026915572,0.000026677093,0.0000212294],"domain_scores_gemma":[0.9981963,0.00057130377,0.00088477164,0.00013515474,0.000066494955,0.00014596399],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049922324,0.00025393718,0.00024396587,0.0008405096,0.00037924698,0.0011730643,0.00043787292,0.00066415704,0.0005741636],"category_scores_gemma":[0.0029831496,0.00019365046,0.00021982339,0.0014590167,0.0010491522,0.00097011705,0.001173241,0.000494221,0.00010107613],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034332197,0.00009550852,0.9048502,0.00015493517,0.00008899402,0.0022151044,0.0010349225,0.011750114,0.010188766,0.033609502,0.00092351483,0.034745213],"study_design_scores_gemma":[0.00004010147,0.00016164097,0.93617225,0.00005538802,0.00004346038,0.0032914735,0.0010701407,0.017971514,0.0015683249,0.035044037,0.0045368737,0.0000447759],"about_ca_topic_score_codex":0.0029805196,"about_ca_topic_score_gemma":0.0021535852,"teacher_disagreement_score":0.0029805196,"about_ca_system_score_codex":0.00040791693,"about_ca_system_score_gemma":0.00008421347,"threshold_uncertainty_score":0.0059263706},"labels":[],"label_agreement":null},{"id":"W2042426607","doi":"10.1086/319041","title":"The Search for Cosmological Black Holes: A Surface Brightness Variability Test","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Gravitational microlensing; Dark matter; Quasar; Galaxy; Population; Surface brightness; Universe; Redshift","score_opus":0.015020714425617865,"score_gpt":0.24642796819201493,"score_spread":0.23140725376639706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042426607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913191,0.0003329862,0.0026114278,0.0021119064,0.00002094019,0.000016586553,0.00020093026,0.000023645529,0.00336249],"genre_scores_gemma":[0.99918383,0.000031496256,0.00034769875,0.00014407412,0.000060641243,0.0000065840604,0.00007718715,0.0000052857617,0.00014312945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99743134,0.0013084909,0.00009114581,0.00046620014,0.00042428498,0.00027856004],"domain_scores_gemma":[0.9183774,0.062013734,0.0116116805,0.003856461,0.0008076669,0.0033330785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0062026177,0.00040622114,0.00063583447,0.0010210552,0.00075624615,0.0014854501,0.0013981075,0.0018804427,0.005448481],"category_scores_gemma":[0.040818337,0.00019261554,0.0007903087,0.0009780681,0.0031055238,0.0023251052,0.0017929726,0.0013429379,0.0003739776],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017978047,0.00039832862,0.9523267,0.000064705135,0.00072482805,0.0009929917,0.0006624157,0.0013705958,0.003912618,0.015540634,0.0010150262,0.021193305],"study_design_scores_gemma":[0.00045775407,0.0013767311,0.89973867,0.000039352573,0.00039377183,0.0025362987,0.0015484032,0.029843215,0.0028368772,0.0588019,0.0023673743,0.000059759084],"about_ca_topic_score_codex":0.00067494175,"about_ca_topic_score_gemma":0.00041232066,"teacher_disagreement_score":0.0062026177,"about_ca_system_score_codex":0.0002389592,"about_ca_system_score_gemma":0.00035889877,"threshold_uncertainty_score":0.032803},"labels":[],"label_agreement":null},{"id":"W2042439050","doi":"10.1088/0004-637x/775/2/90","title":"THE DYNAMICS OF STAR STREAM GAPS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; RADIUS; STREAMS; Relative velocity; Angular momentum; Mechanics; Orbit (dynamics); Classical mechanics; Computational physics; Astrophysics","score_opus":0.004335247640620685,"score_gpt":0.1948982956223158,"score_spread":0.19056304798169513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042439050","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9918343,0.0001355727,0.00389917,0.00016485661,0.000013878088,0.000009427452,0.000103209895,0.000057270518,0.0037823226],"genre_scores_gemma":[0.9983577,0.000060786326,0.00060544786,0.000009053349,0.0000054846387,0.0000063416055,0.000056401335,0.000014410271,0.000884346],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987555,0.000014962906,0.000008986126,0.000025795413,0.000030115183,0.000044534358],"domain_scores_gemma":[0.99891555,0.00026951893,0.00030560105,0.000074242715,0.00014031348,0.00029485713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030146187,0.00014596817,0.00027792653,0.00050572376,0.0005776987,0.0011702157,0.00035946563,0.00065416365,0.0021347255],"category_scores_gemma":[0.0027665906,0.00022725452,0.00026092923,0.00020693899,0.0006800016,0.0012951894,0.0009949673,0.0006385475,0.00027820544],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010754841,0.00032331733,0.2007103,0.00016906713,0.000072109164,0.0036692824,0.0035210599,0.38928935,0.07125186,0.27798006,0.0042302515,0.047707755],"study_design_scores_gemma":[0.00006620388,0.00027889627,0.08116487,0.00006952341,0.000023084507,0.0012590174,0.0012817408,0.8377533,0.012317445,0.05759407,0.00812082,0.00007098462],"about_ca_topic_score_codex":0.0020578043,"about_ca_topic_score_gemma":0.0009947063,"teacher_disagreement_score":0.0021347255,"about_ca_system_score_codex":0.0009824084,"about_ca_system_score_gemma":0.0004502027,"threshold_uncertainty_score":0.007141292},"labels":[],"label_agreement":null},{"id":"W2042541725","doi":"10.1086/500207","title":"A Local Group Polar Ring Galaxy: NGC 6822","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Stellar population; Galaxy; Rotation (mathematics); Thick disk; Velocity dispersion; Local Group; Polar; Stars; Population; Galaxy rotation curve; Astronomy; Dwarf galaxy; Star formation; Geometry; Galaxy formation and evolution; Halo","score_opus":0.008377160483087726,"score_gpt":0.2150458745084905,"score_spread":0.20666871402540277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042541725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98167276,0.00019790619,0.00026540723,0.000056342127,0.000010871643,0.000021670077,0.0015512797,0.00015239122,0.016071301],"genre_scores_gemma":[0.9917542,0.00007462074,0.00028876017,0.000024995006,0.000022778058,0.000009127769,0.0015576879,0.000012088917,0.006255699],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999596,0.000003906514,0.0000011072077,0.000014093317,0.0000069752214,0.000014308513],"domain_scores_gemma":[0.99994516,0.0000033481933,0.000014872042,0.000006725138,0.000007425211,0.000022464146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000039756284,0.000248864,0.0001152301,0.00053617446,0.00046067944,0.00027443582,0.00016263202,0.00016799968,0.010467752],"category_scores_gemma":[0.000102054706,0.000054046584,0.00004975229,0.00049569964,0.0001228702,0.0001784259,0.00026206736,0.00009231843,0.0038228086],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003744303,0.00020707469,0.8218973,0.00014867059,0.000047541726,0.003194453,0.0025683478,0.00036176445,0.04769426,0.0011544562,0.024264224,0.09808744],"study_design_scores_gemma":[0.00001860615,0.00017007814,0.9618503,0.000015073196,0.000017636643,0.0033224504,0.0007097573,0.0003351291,0.0010886298,0.00011928686,0.03234575,0.000007372703],"about_ca_topic_score_codex":0.007221508,"about_ca_topic_score_gemma":0.012419211,"teacher_disagreement_score":0.010467752,"about_ca_system_score_codex":0.00018640679,"about_ca_system_score_gemma":0.000071963885,"threshold_uncertainty_score":0.035018086},"labels":[],"label_agreement":null},{"id":"W2042739420","doi":"10.1088/0004-637x/775/1/53","title":"TESTING IN SITU ASSEMBLY WITH THE<i>KEPLER</i>PLANET CANDIDATE SAMPLE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":263,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Monte Carlo method; RADIUS; Mass distribution; Solar System; Range (aeronautics); Terrestrial planet; Planetary system; Dissipation","score_opus":0.011631472407373958,"score_gpt":0.21159014341602536,"score_spread":0.1999586710086514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042739420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931606,0.000015522608,0.005576685,0.00008120113,0.000004642062,0.000024245544,0.00024600467,0.00009016547,0.0008009878],"genre_scores_gemma":[0.99510443,0.0000120593495,0.0037698736,0.000023835877,0.000005092832,0.000025142497,0.0006946252,0.000027478864,0.00033750848],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986737,0.00076440757,0.000043794138,0.00030252672,0.00014147359,0.000074197495],"domain_scores_gemma":[0.97965723,0.015582938,0.0015040745,0.0019250582,0.00079138984,0.00053922914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004092986,0.00036340105,0.00030972104,0.00037810998,0.0004811014,0.0009856584,0.0013451248,0.00075834227,0.0026784255],"category_scores_gemma":[0.020048415,0.00036194202,0.00061097887,0.00041938375,0.00047918668,0.00087636866,0.000882669,0.0004765057,0.000567194],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016995762,0.0005780019,0.7834718,0.00006266859,0.0003616578,0.00031636903,0.0006522627,0.18307003,0.008893811,0.0027779834,0.00089493283,0.017220816],"study_design_scores_gemma":[0.00016998325,0.0010135756,0.109337196,0.000013645942,0.00015799595,0.00044104643,0.0003792673,0.8665593,0.018127248,0.0019593337,0.0018128054,0.000028612845],"about_ca_topic_score_codex":0.0040139444,"about_ca_topic_score_gemma":0.0037632252,"teacher_disagreement_score":0.004092986,"about_ca_system_score_codex":0.00060740084,"about_ca_system_score_gemma":0.0004565241,"threshold_uncertainty_score":0.021646082},"labels":[],"label_agreement":null},{"id":"W2042829205","doi":"10.1086/587453","title":"Accretion‐powered Stellar Winds. III. Spin‐Equilibrium Solutions","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Stellar atmosphere; Stellar evolution; Computational astrophysics; Stars; Stellar physics; Stellar structure; Stellar rotation","score_opus":0.019950226620184697,"score_gpt":0.24313628082057584,"score_spread":0.22318605420039114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042829205","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14627013,0.026579138,0.14709207,0.014209519,0.003622258,0.00031136782,0.0013619099,0.0004756264,0.6600779],"genre_scores_gemma":[0.8255238,0.008863174,0.012542688,0.0018576345,0.0027787217,0.00025440287,0.0006444429,0.00024187296,0.1472933],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998534,0.00003242527,0.000008095494,0.0000167274,0.000044375534,0.000045011548],"domain_scores_gemma":[0.99976164,0.000039821727,0.000049355465,0.000026842345,0.000059320962,0.0000630256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038199426,0.00083617476,0.0007485222,0.0008933537,0.0009198915,0.0024064425,0.0013881861,0.0020205067,0.0067177597],"category_scores_gemma":[0.0016289016,0.0005109658,0.0010170896,0.00048613836,0.0014470195,0.001630669,0.0020017342,0.0014158398,0.0024492445],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036599053,0.000025496074,0.00043833815,0.00009645141,0.00002441559,0.00026047794,0.00010651364,0.03582233,0.0010626389,0.94498074,0.0088850465,0.008261052],"study_design_scores_gemma":[0.00007816054,0.000034517358,0.0009786421,0.00008677414,0.000014082046,0.0002962128,0.00014359687,0.17949693,0.00032910175,0.8080608,0.0104515385,0.000029649425],"about_ca_topic_score_codex":0.0037152201,"about_ca_topic_score_gemma":0.0023977333,"teacher_disagreement_score":0.0067177597,"about_ca_system_score_codex":0.00096113415,"about_ca_system_score_gemma":0.0008091878,"threshold_uncertainty_score":0.022473156},"labels":[],"label_agreement":null},{"id":"W2042926361","doi":"10.1086/429794","title":"The T Tauri Phase Down to Nearly Planetary Masses: Echelle Spectra of 82 Very Low Mass Stars and Brown Dwarfs","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":335,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Low Mass; Accretion (finance); Spectral line; T Tauri star; Stars; Stellar classification; Accretion disc","score_opus":0.007092417408848139,"score_gpt":0.23427565194716707,"score_spread":0.22718323453831893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042926361","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994777,0.000022902464,0.00007796071,0.0000035680705,3.6620028e-7,0.0000014073064,0.00020091848,0.0000047606977,0.00021045296],"genre_scores_gemma":[0.99883324,0.000021085356,0.00026404636,0.0000064759356,0.0000029585133,0.000003042104,0.00065811863,0.0000036906474,0.00020731207],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990153,0.00001301629,0.000009315622,0.00003056095,0.000021532149,0.000024020299],"domain_scores_gemma":[0.99954766,0.00010101075,0.00012752698,0.000039843515,0.00006737641,0.000116645824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022911862,0.0001694804,0.00018129876,0.00081139564,0.00023123865,0.00032830995,0.00014126001,0.00017305897,0.0006084809],"category_scores_gemma":[0.00038223102,0.00010077433,0.00012386318,0.00056932366,0.00013110529,0.0001896167,0.00039894794,0.00013203744,0.00030562736],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003246771,0.000070461494,0.95676607,0.000016791755,0.000026318616,0.00024252657,0.00060016033,0.00018753695,0.03341148,0.00006278048,0.00014960706,0.0081416555],"study_design_scores_gemma":[0.0000031156299,0.000045463436,0.9982981,0.000001169264,0.000004954663,0.0001951931,0.00009957288,0.00015962706,0.00096725184,0.00001484528,0.00020919046,0.0000014619274],"about_ca_topic_score_codex":0.0017056438,"about_ca_topic_score_gemma":0.0024879705,"teacher_disagreement_score":0.0017056438,"about_ca_system_score_codex":0.000106999636,"about_ca_system_score_gemma":0.00005798025,"threshold_uncertainty_score":0.0033914447},"labels":[],"label_agreement":null},{"id":"W2042939888","doi":"10.1088/0004-637x/757/2/123","title":"CONSTRAINTS ON COSMIC RAYS, MAGNETIC FIELDS, AND DARK MATTER FROM GAMMA-RAY OBSERVATIONS OF THE COMA CLUSTER OF GALAXIES WITH VERITAS AND<i>FERMI</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Coma Cluster; Astrophysics; Radio halo; Cosmic ray; Galaxy; Fermi Gamma-ray Space Telescope; Galaxy cluster; Fermi acceleration; Coma (optics); Dark matter; Electron; Astronomy; Particle acceleration; Nuclear physics","score_opus":0.008989487584946507,"score_gpt":0.19374606780039713,"score_spread":0.18475658021545063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042939888","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9771435,0.0004440182,0.010496328,0.00011394345,0.000009003441,0.0000106510815,0.0012122113,0.00015458048,0.010415867],"genre_scores_gemma":[0.9970282,0.000112379734,0.0016255326,0.000022676133,0.0000060773,0.000005952115,0.00091488025,0.000010669331,0.00027369353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977213,0.000038735634,0.000013549165,0.000051789684,0.00006620869,0.000057480607],"domain_scores_gemma":[0.9990759,0.00031606603,0.0002630274,0.00016406503,0.000088924564,0.00009200721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006308173,0.00069501216,0.0002702701,0.00079788367,0.0004435086,0.0006677461,0.0004118422,0.00018653926,0.0034029668],"category_scores_gemma":[0.001868142,0.00022030514,0.00036353496,0.000589149,0.0005061033,0.0004362585,0.00087172614,0.0002992772,0.0003445057],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007406141,0.0000683941,0.83608,0.00024310681,0.000389991,0.00036570217,0.00037702918,0.03317884,0.055877827,0.025904568,0.0021571876,0.04461673],"study_design_scores_gemma":[0.00003659429,0.00016358231,0.94666344,0.000067365894,0.00009524389,0.00027386157,0.00017911787,0.023102896,0.018530872,0.0058298158,0.0050179646,0.000039279526],"about_ca_topic_score_codex":0.01615682,"about_ca_topic_score_gemma":0.028520657,"teacher_disagreement_score":0.01615682,"about_ca_system_score_codex":0.0006965021,"about_ca_system_score_gemma":0.00042295418,"threshold_uncertainty_score":0.032125533},"labels":[],"label_agreement":null},{"id":"W2042991161","doi":"10.1086/592379","title":"Discovery of a Wide Substellar Companion to a Nearby Low‐Mass Star","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Sky; Metallicity; Brown dwarf; Primary (astronomy); Proper motion; Binary number; Globular cluster; Low Mass; Solar mass","score_opus":0.011960184508441487,"score_gpt":0.21478630159812517,"score_spread":0.20282611708968368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2042991161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937195,0.00007481159,0.00012911683,0.000019465379,0.0000027875142,0.0000018996437,0.000025961695,0.000010649314,0.0003633105],"genre_scores_gemma":[0.999496,0.000023288569,0.00020027727,0.00003084884,0.0000054943334,0.0000011829336,0.00008972975,0.0000010390683,0.00015217935],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999199,0.000005441217,0.000005097361,0.000027140732,0.00001996457,0.000022440006],"domain_scores_gemma":[0.9997018,0.00003504507,0.00010745412,0.000032337786,0.000017944116,0.0001053193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015115447,0.00012516756,0.00016776468,0.000398781,0.0005271562,0.00042874168,0.0003325935,0.00048674765,0.000668935],"category_scores_gemma":[0.00030379108,0.00011918349,0.00011713572,0.00024266628,0.00026373926,0.00016287906,0.0004849057,0.00020697608,0.00030885148],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027277725,0.000095637006,0.84316033,0.00004912119,0.000044920274,0.011208516,0.00077332783,0.00013220972,0.12822539,0.0003813762,0.0004820451,0.015174358],"study_design_scores_gemma":[0.000015097978,0.00057687925,0.96438587,0.0000060540256,0.000041290044,0.017880391,0.000287063,0.0005849208,0.0126698185,0.00022276105,0.0033191238,0.000010669539],"about_ca_topic_score_codex":0.0013477942,"about_ca_topic_score_gemma":0.0024666158,"teacher_disagreement_score":0.0013477942,"about_ca_system_score_codex":0.0002127664,"about_ca_system_score_gemma":0.0001589989,"threshold_uncertainty_score":0.0026798844},"labels":[],"label_agreement":null},{"id":"W2043020462","doi":"10.1086/588138","title":"A <i>z</i> = 0.9 Supercluster of X-Ray Luminous, Optically Selected, Massive Galaxy Clusters","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Supercluster (genetic); Redshift; Galaxy cluster; Galaxy; Cluster (spacecraft); Astronomy; Line-of-sight; Galaxy groups and clusters; Chemistry","score_opus":0.006677624261415365,"score_gpt":0.19398636787197215,"score_spread":0.1873087436105568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043020462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864215,0.000077529934,0.00021343649,0.0000134856655,0.0000025961683,0.0000048722372,0.00019416663,0.000026152395,0.00082565023],"genre_scores_gemma":[0.9985713,0.000023924918,0.00049347244,0.000010360879,0.000005934825,0.000002708251,0.0006888393,0.0000035960197,0.00019989476],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999218,0.0000028742904,0.0000043535506,0.000030431214,0.000019436138,0.000021080776],"domain_scores_gemma":[0.9997465,0.00001630748,0.00011581322,0.00003342949,0.00002398174,0.000063952524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007730495,0.00013099432,0.00014745425,0.00056569395,0.00032562483,0.0005288656,0.0002630183,0.000096448246,0.000857421],"category_scores_gemma":[0.00025923536,0.00010330072,0.000096626005,0.00045270147,0.00030476638,0.00016718676,0.00043299288,0.000108859334,0.00018766406],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078416406,0.00007976344,0.72842705,0.00006814036,0.00009828058,0.0011742511,0.0006208924,0.0013080954,0.24728447,0.0023370772,0.0012642153,0.016553532],"study_design_scores_gemma":[0.000020374566,0.000087312466,0.98335224,0.000007879952,0.000032494256,0.0013182067,0.00012164462,0.0024198801,0.010504926,0.000474356,0.0016508357,0.000009746128],"about_ca_topic_score_codex":0.0027979615,"about_ca_topic_score_gemma":0.0026213103,"teacher_disagreement_score":0.0027979615,"about_ca_system_score_codex":0.00027737222,"about_ca_system_score_gemma":0.00011490083,"threshold_uncertainty_score":0.0055633783},"labels":[],"label_agreement":null},{"id":"W2043051302","doi":"10.1086/591779","title":"The DEEP2 Redshift Survey: Lyα Emitters in the Spectroscopic Database","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Redshift; Astrophysics; Narrowband; Sky; Physics; Line (geometry); Quality (philosophy); Component (thermodynamics); Database; Astronomy; Computer science; Optics; Galaxy","score_opus":0.01429132716981101,"score_gpt":0.23101009088725002,"score_spread":0.216718763717439,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043051302","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9768793,0.0007583491,0.0037448069,0.0001253718,0.000010618103,0.00005083055,0.015001923,0.0001602851,0.0032685255],"genre_scores_gemma":[0.9587856,0.0003121905,0.00783475,0.00015114396,0.000029388411,0.0000508389,0.031070255,0.00006772933,0.0016981415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994628,0.00007998606,0.000047026402,0.00012383735,0.0001518232,0.00013458001],"domain_scores_gemma":[0.9972434,0.0003146111,0.0007450925,0.00044100083,0.00050781254,0.00074803864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013084831,0.0004094523,0.0004023778,0.0039264583,0.00046897854,0.0009609817,0.0006427795,0.0003016502,0.0030390483],"category_scores_gemma":[0.002194214,0.0002174457,0.0002710029,0.002841045,0.0001794051,0.0008316708,0.0018601649,0.00031529498,0.00094170304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042584608,0.00016075134,0.9106451,0.00019454754,0.00015753783,0.00026078537,0.00053971267,0.0005716805,0.028319718,0.00085087057,0.0054116333,0.052461844],"study_design_scores_gemma":[0.00004118362,0.0000993865,0.9754233,0.00002623641,0.00007165468,0.0006154659,0.0003141092,0.0013880319,0.004420309,0.0004161541,0.017163968,0.000020173175],"about_ca_topic_score_codex":0.0046359366,"about_ca_topic_score_gemma":0.009956657,"teacher_disagreement_score":0.0046359366,"about_ca_system_score_codex":0.00033833904,"about_ca_system_score_gemma":0.00038770703,"threshold_uncertainty_score":0.010166705},"labels":[],"label_agreement":null},{"id":"W2043262952","doi":"10.1086/319814","title":"Ultraviolet Line Spectra of Metal‐poor Star‐forming Galaxies","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Metallicity; Physics; Astrophysics; Spectral line; Galaxy; Stars; Astronomy; Ultraviolet; Redshift","score_opus":0.009420821549491405,"score_gpt":0.22095354610680865,"score_spread":0.21153272455731725,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043262952","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98801106,0.00007817062,0.004317105,0.000037821064,0.000008179988,0.000017784814,0.004993324,0.0006386056,0.0018979887],"genre_scores_gemma":[0.98902076,0.00005554319,0.0041220314,0.000023377565,0.0000067347996,0.00001635916,0.0063396273,0.000081415616,0.0003340973],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999038,0.000020796648,0.0000060543166,0.000035396806,0.000019200528,0.000014729856],"domain_scores_gemma":[0.99962413,0.000090571986,0.00008203226,0.000086637054,0.00005491201,0.00006169968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027203813,0.0003489346,0.0001994317,0.00075929234,0.00015891812,0.00037297764,0.0003771549,0.0003412807,0.0012341177],"category_scores_gemma":[0.00053012563,0.00018068009,0.00057330535,0.0007080039,0.00013465247,0.00021509253,0.0001889055,0.00022211565,0.0003564077],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096418697,0.00054138544,0.5258628,0.0003775448,0.000572936,0.00077689276,0.00064367,0.33842888,0.083338894,0.004106219,0.0079272725,0.036459308],"study_design_scores_gemma":[0.00015862932,0.00025276616,0.64066017,0.000026883157,0.00014892865,0.00057838066,0.00014192237,0.32867414,0.020753948,0.0022123945,0.006335767,0.000056098546],"about_ca_topic_score_codex":0.0025439712,"about_ca_topic_score_gemma":0.0023137995,"teacher_disagreement_score":0.0025439712,"about_ca_system_score_codex":0.0004028353,"about_ca_system_score_gemma":0.000068944755,"threshold_uncertainty_score":0.005058348},"labels":[],"label_agreement":null},{"id":"W2043302786","doi":"10.1088/0004-637x/731/1/4","title":"THE SHAPE AND PROFILE OF THE MILKY WAY HALO AS SEEN BY THE CANADA-FRANCE-HAWAII TELESCOPE LEGACY SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":172,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Halo; Milky Way; Metallicity; Stars; Galactic halo; Sagittarius; Astronomy; Galaxy","score_opus":0.012032478445668557,"score_gpt":0.20364339730589748,"score_spread":0.1916109188602289,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043302786","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996534,0.00006505003,0.00008505105,0.000026758109,0.0000012515185,0.000004064797,0.0016851483,0.000026920567,0.0015716606],"genre_scores_gemma":[0.9971106,0.000065004046,0.00017483869,0.000013215305,0.000002053532,0.0000035546266,0.00217025,0.000009420553,0.00045103725],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991715,0.0000108389095,0.0000035200833,0.00001994263,0.000024782556,0.000023682256],"domain_scores_gemma":[0.9991887,0.000078064695,0.00019102801,0.00008045936,0.00020311607,0.000258616],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022408154,0.00014292776,0.00014676117,0.0012042732,0.00025563056,0.0006673272,0.00026351254,0.00018674179,0.0013168254],"category_scores_gemma":[0.0008681385,0.0001248731,0.00021654944,0.0010467601,0.0002658944,0.00020979866,0.00035975277,0.00013125238,0.00025904857],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000025120708,0.00000821832,0.99320626,0.0000081134995,0.00004927777,0.000058593065,0.00026844532,0.0011312722,0.002306279,0.0001470938,0.0005197728,0.0022716585],"study_design_scores_gemma":[0.0000010989755,0.0000040712835,0.9989479,0.0000023966916,0.0000041587864,0.000019731997,0.000088355635,0.0005063319,0.00006880409,0.000013998168,0.00034003385,0.0000031754787],"about_ca_topic_score_codex":0.25065538,"about_ca_topic_score_gemma":0.34401006,"teacher_disagreement_score":0.25065538,"about_ca_system_score_codex":0.0012517811,"about_ca_system_score_gemma":0.00055838254,"threshold_uncertainty_score":0.49839282},"labels":[],"label_agreement":null},{"id":"W2043467481","doi":"10.1086/341734","title":"The Transport of Charged Particles in a Flowing Medium","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Scattering; Pitch angle; Anisotropy; Adiabatic process; Computational physics; Isotropy; Classical mechanics; Forward scatter; Optics; Quantum mechanics","score_opus":0.00917393052992943,"score_gpt":0.20737589479070678,"score_spread":0.19820196426077735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043467481","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34454042,0.002576667,0.6315084,0.0007091722,0.0007662914,0.00015873996,0.0003674705,0.0004453994,0.01892747],"genre_scores_gemma":[0.89344466,0.001981096,0.0843402,0.00019316445,0.00023407968,0.00012989019,0.0003343717,0.00011335741,0.019229168],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.999926,0.000013917743,0.0000038465646,0.000015314074,0.00002610025,0.000014856193],"domain_scores_gemma":[0.9998747,0.000041500978,0.00002296978,0.000010642081,0.00003260367,0.000017464125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024969465,0.0005758947,0.0003576698,0.0005718943,0.0006500237,0.00081370026,0.0006810062,0.0007374915,0.00091877294],"category_scores_gemma":[0.00056094705,0.0002820717,0.00061088597,0.00038848602,0.0006368452,0.001196302,0.00060385896,0.0005447514,0.00020892751],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012980074,0.00010881436,0.0033570686,0.00029818065,0.000105459156,0.001319018,0.0003621425,0.45329362,0.15067635,0.35992995,0.00197524,0.028444404],"study_design_scores_gemma":[0.00002859601,0.000055358527,0.0005167635,0.000009599066,0.000014609482,0.00014569293,0.000028698516,0.97711253,0.0049642944,0.014621065,0.0024692763,0.000033484488],"about_ca_topic_score_codex":0.0030248684,"about_ca_topic_score_gemma":0.0013224713,"teacher_disagreement_score":0.0030248684,"about_ca_system_score_codex":0.0008392903,"about_ca_system_score_gemma":0.000780075,"threshold_uncertainty_score":0.0060895085},"labels":[],"label_agreement":null},{"id":"W2043584675","doi":"10.1086/506439","title":"Removing the Microlensing Blending‐Parallax Degeneracy Using Source Variability","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gravitational microlensing; Degeneracy (biology); Physics; Parallax; Halo; Lens (geology); Gravitational lens; Astrophysics; Variable star; Microlens; Event (particle physics); Stars; Star (game theory); Astronomy; Optics; Galaxy","score_opus":0.0109494644233933,"score_gpt":0.22340726525914525,"score_spread":0.21245780083575194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043584675","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9526978,0.00012806297,0.04180378,0.00017152252,0.000028167167,0.000015383519,0.0002379282,0.00031138174,0.0046060095],"genre_scores_gemma":[0.98642737,0.00006172321,0.012546727,0.00003604663,0.000022958346,0.0000059401236,0.00039573663,0.000045128687,0.0004583711],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997532,0.000026484653,0.000015250497,0.000066382316,0.00008424257,0.00005440344],"domain_scores_gemma":[0.9987185,0.000502094,0.000251134,0.00037020497,0.000056983343,0.00010111715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003081497,0.00030018674,0.00053260534,0.00047790873,0.00048550346,0.0009351741,0.00041048703,0.00038119178,0.0018425602],"category_scores_gemma":[0.0031677508,0.00015287676,0.00042781045,0.00055152265,0.00019802366,0.00069894537,0.0007922748,0.0005980381,0.0004063995],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007521875,0.00038070546,0.33900505,0.00015472223,0.00031070644,0.0013536715,0.0004218102,0.026874479,0.16112524,0.01856219,0.0018768596,0.4491824],"study_design_scores_gemma":[0.00017736881,0.0003326005,0.45691228,0.000045461333,0.0004253526,0.0022206125,0.0002617786,0.4129839,0.07531302,0.04336735,0.007865798,0.00009450517],"about_ca_topic_score_codex":0.0009557383,"about_ca_topic_score_gemma":0.0021215735,"teacher_disagreement_score":0.0018425602,"about_ca_system_score_codex":0.000115479575,"about_ca_system_score_gemma":0.0003011522,"threshold_uncertainty_score":0.0061639547},"labels":[],"label_agreement":null},{"id":"W2043685525","doi":"10.1086/427920","title":"Dead Zones and the Origin of Planetary Masses","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Planet; Protoplanet; Jovian; Planetary migration; Gas giant; Planetary system; Solar System; Formation and evolution of the Solar System; Planetary mass","score_opus":0.009995449875641469,"score_gpt":0.23035280629083407,"score_spread":0.2203573564151926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043685525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932433,0.001250181,0.00082623604,0.0001811308,0.000005301589,0.0000027446479,0.00008423999,0.000018633515,0.004388155],"genre_scores_gemma":[0.9993536,0.00012921302,0.00011965178,0.000009525094,0.000004547452,6.5591837e-7,0.000045205765,0.0000046193986,0.00033299043],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99989164,0.000016834945,0.000008149439,0.000026804084,0.000023631657,0.000033002365],"domain_scores_gemma":[0.9978288,0.0005390939,0.0009174535,0.00016147991,0.000102732185,0.00045040366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027707595,0.00013690561,0.00016695498,0.00087988947,0.0007929735,0.0017971984,0.00060526695,0.00045560635,0.0023283693],"category_scores_gemma":[0.0038438507,0.00016534049,0.00012720838,0.00044054707,0.0015036559,0.001251877,0.0013743954,0.0006018451,0.00031733813],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011737425,0.00010405621,0.75887644,0.00021175382,0.00011339339,0.0013535073,0.008313351,0.0063509033,0.031298637,0.13994652,0.0012722721,0.05098534],"study_design_scores_gemma":[0.00004872329,0.000109362794,0.88294345,0.000057274225,0.00005560258,0.002032776,0.002761022,0.004216404,0.007475306,0.08226276,0.017988242,0.00004916607],"about_ca_topic_score_codex":0.0011576379,"about_ca_topic_score_gemma":0.000964877,"teacher_disagreement_score":0.0023283693,"about_ca_system_score_codex":0.0005075384,"about_ca_system_score_gemma":0.000110499015,"threshold_uncertainty_score":0.007789135},"labels":[],"label_agreement":null},{"id":"W2043694847","doi":"10.1086/510670","title":"ACS Photometry of Extended, Luminous Globular Clusters in the Outskirts of M31","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Horizontal branch; Photometry (optics); Luminosity; Star cluster; Galaxy; Stellar population; Milky Way","score_opus":0.005475828682587897,"score_gpt":0.2105325312836229,"score_spread":0.205056702601035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043694847","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990369,0.000034756344,0.0000687127,0.0000058848887,6.9385555e-7,0.0000038299945,0.000117001684,0.000007979265,0.00072435295],"genre_scores_gemma":[0.9985014,0.00005210225,0.00034663107,0.000009672042,0.0000052559367,0.000004820419,0.00070918474,0.00000566824,0.00036531722],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987864,0.000009206898,0.000008904606,0.000027879823,0.00004031722,0.000035004363],"domain_scores_gemma":[0.9995301,0.000037688256,0.00012442697,0.000051953233,0.00008833093,0.00016760667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016282675,0.00020843526,0.00023167515,0.0015277228,0.00045262664,0.00054081023,0.00022219507,0.00018590571,0.0007014083],"category_scores_gemma":[0.000662275,0.00015407868,0.00013549469,0.0009171042,0.00024420998,0.0002804534,0.0007717207,0.00015511912,0.00023521586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020737438,0.00004365344,0.93583363,0.000027424307,0.00002096759,0.00055964635,0.0012410064,0.000659617,0.047936052,0.00043525652,0.0005820547,0.012453368],"study_design_scores_gemma":[0.0000025599677,0.000014718144,0.9985506,0.0000023803314,0.0000035648561,0.00015418621,0.00009049949,0.00027490727,0.0004737662,0.0000440886,0.0003861864,0.0000026199507],"about_ca_topic_score_codex":0.0111711025,"about_ca_topic_score_gemma":0.022957146,"teacher_disagreement_score":0.0111711025,"about_ca_system_score_codex":0.00039325212,"about_ca_system_score_gemma":0.0001751542,"threshold_uncertainty_score":0.022212148},"labels":[],"label_agreement":null},{"id":"W2043714894","doi":"10.1086/320963","title":"Forces on Dust Grains Exposed to Anisotropic Interstellar Radiation Fields","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Anisotropy; Photoelectric effect; Physics; Radiation; Radiation pressure; Absorption (acoustics); Interstellar medium; Cosmic dust; Starlight; Photon; Scattering; Radiation damage; Astrophysics; Stars; Computational physics; Atomic physics; Optics; Galaxy","score_opus":0.014005958475903607,"score_gpt":0.24400531345020232,"score_spread":0.22999935497429871,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043714894","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99677426,0.00007965049,0.0009071928,0.00004847134,0.000010133456,0.000008788429,0.000058563077,0.000019922898,0.0020929577],"genre_scores_gemma":[0.9992204,0.00006977104,0.00016812937,0.000009730484,0.0000066484913,0.0000043035247,0.00005216881,0.0000070490523,0.00046181487],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999105,0.00000669423,0.00000398439,0.00001980114,0.00002466088,0.00003440471],"domain_scores_gemma":[0.9998373,0.000033177348,0.000046260026,0.000013491829,0.0000228926,0.000046863297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008717286,0.0002554985,0.00032722097,0.00058401807,0.0007682999,0.00082412554,0.00033155098,0.00037545292,0.0015440396],"category_scores_gemma":[0.00048116356,0.00019797834,0.00030979427,0.00022130896,0.0006691939,0.00042241122,0.0006916543,0.00023517259,0.00019755066],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013191428,0.00047934323,0.16954179,0.00030609537,0.00033878357,0.005892855,0.0013355839,0.32062286,0.44257537,0.020867473,0.0019298677,0.034790907],"study_design_scores_gemma":[0.000538335,0.00085155125,0.361416,0.00004464938,0.00019132158,0.0012312363,0.0019926168,0.55730414,0.060044855,0.011527792,0.004679719,0.0001777547],"about_ca_topic_score_codex":0.006369679,"about_ca_topic_score_gemma":0.00230819,"teacher_disagreement_score":0.006369679,"about_ca_system_score_codex":0.00065851415,"about_ca_system_score_gemma":0.00017983808,"threshold_uncertainty_score":0.012665212},"labels":[],"label_agreement":null},{"id":"W2043821096","doi":"10.1088/0004-637x/756/2/147","title":"X-RAY BINARIES IN THE ULTRAHIGH ENCOUNTER RATE GLOBULAR CLUSTER NGC 6388","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Population; Variable star; Binary star; Cluster (spacecraft); RADIUS; Binary number; Light curve; Luminosity","score_opus":0.011812739130754549,"score_gpt":0.23307974983041416,"score_spread":0.2212670106996596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043821096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99988794,0.000007673102,0.00001528549,0.000003647054,2.3929542e-7,7.7143847e-7,0.00002117882,0.0000017888786,0.0000615045],"genre_scores_gemma":[0.9997148,0.00001143409,0.00008128708,0.0000053815597,0.0000012030785,0.0000011946671,0.0000918427,0.0000015653452,0.00009127505],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999879,0.00001370786,0.000007120773,0.000026686266,0.00003339931,0.000040012415],"domain_scores_gemma":[0.99961925,0.000047845795,0.00015013559,0.000047700367,0.00003359419,0.00010142101],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017011716,0.00016326268,0.0002388116,0.0004810303,0.00047593142,0.00036697803,0.00030540104,0.00017614385,0.0005692057],"category_scores_gemma":[0.000430803,0.00013628497,0.00010127778,0.00042382255,0.00028165278,0.00015767543,0.0006803277,0.0002034937,0.00019320894],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023834914,0.000110629844,0.9747785,0.0000091036045,0.000028758606,0.00067615096,0.00066287356,0.0004345894,0.017665336,0.00021576711,0.0002274812,0.004952611],"study_design_scores_gemma":[0.0000075284624,0.00005233659,0.9980203,0.0000018436873,0.0000089987625,0.00047001342,0.000170652,0.00052277657,0.0004028259,0.00007819838,0.0002595099,0.0000050630592],"about_ca_topic_score_codex":0.009114257,"about_ca_topic_score_gemma":0.014542691,"teacher_disagreement_score":0.009114257,"about_ca_system_score_codex":0.00025669078,"about_ca_system_score_gemma":0.00013783274,"threshold_uncertainty_score":0.018122435},"labels":[],"label_agreement":null},{"id":"W2043863877","doi":"10.1086/523659","title":"The Evolution of Galaxy Mergers and Morphology at<i>z</i>&lt; 1.2 in the Extended Groth Strip","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":467,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Galaxy; Galaxy merger; Galaxy formation and evolution; Number density; Elliptical galaxy; Morphology (biology); Lenticular galaxy","score_opus":0.007532605422219067,"score_gpt":0.20504684113220245,"score_spread":0.1975142357099834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043863877","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993731,0.0002590133,0.0001043876,0.00039765536,0.000006537722,0.0000036446736,0.0005548728,0.000031246265,0.0049116598],"genre_scores_gemma":[0.99735475,0.00008422333,0.00010094778,0.00009428968,0.000022493883,0.0000036433626,0.000858738,0.0000249191,0.001456006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987936,0.000014830841,0.0000028826782,0.000033274755,0.000022163822,0.00004744665],"domain_scores_gemma":[0.9990528,0.00015449109,0.00029939684,0.000054443623,0.00011410931,0.00032479202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035250108,0.00015448412,0.00024389492,0.0011612633,0.0005857454,0.0016565092,0.0003333776,0.0006348478,0.0042312318],"category_scores_gemma":[0.0010947713,0.00021902734,0.00023033733,0.0009813799,0.000532086,0.00065268995,0.0010483708,0.0006670652,0.0010247754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005988759,0.00010725342,0.927741,0.00005626002,0.00013832543,0.0008499974,0.0028984507,0.002985808,0.0271905,0.006942881,0.007279571,0.023210935],"study_design_scores_gemma":[0.000005103569,0.000013856133,0.998329,0.0000044312806,0.0000055089195,0.00004669765,0.00014683316,0.00028281164,0.00013474927,0.00020786688,0.00081754004,0.0000055667915],"about_ca_topic_score_codex":0.009691647,"about_ca_topic_score_gemma":0.016022116,"teacher_disagreement_score":0.009691647,"about_ca_system_score_codex":0.00057714095,"about_ca_system_score_gemma":0.0001678218,"threshold_uncertainty_score":0.01927048},"labels":[],"label_agreement":null},{"id":"W2043889033","doi":"10.1088/0004-637x/779/1/88","title":"MULTIWAVELENGTH OBSERVATIONS OF THE TeV BINARY LS I +61° 303 WITH VERITAS,<i>Fermi</i>-LAT, AND<i>Swift</i>/XRT DURING A TeV OUTBURST","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Binary number; Telescope; Fermi Gamma-ray Space Telescope; Satellite; Spectral energy distribution; Spectral line; High energy; Energy spectrum","score_opus":0.009386793579931696,"score_gpt":0.19327202235872723,"score_spread":0.18388522877879554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043889033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990196,0.000038014812,0.0000540995,0.000016545566,0.000002310521,0.000002709581,0.00030640277,0.000011570005,0.00054876314],"genre_scores_gemma":[0.9986045,0.00002709495,0.0003208723,0.000019872754,0.0000072471503,0.0000037493237,0.00080043497,0.0000063552284,0.00020997532],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984515,0.000012978396,0.0000079310075,0.000039521692,0.000046721045,0.000047645262],"domain_scores_gemma":[0.99948955,0.000055238957,0.00021394626,0.000050002185,0.00005405917,0.00013710644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023756709,0.00015250752,0.00022997195,0.00062170945,0.00046121902,0.0003980664,0.00026555773,0.00028362364,0.00078474294],"category_scores_gemma":[0.00030675504,0.00021361261,0.00019413373,0.0005715289,0.00022071134,0.00018607047,0.0005630707,0.00042759575,0.00022698862],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076421304,0.00012861172,0.8671578,0.000048401584,0.00010803134,0.00084032177,0.000923911,0.0006917082,0.1144748,0.0002478486,0.0011616885,0.013452638],"study_design_scores_gemma":[0.000008709277,0.000051714484,0.9979911,0.0000041873614,0.000012754099,0.0001627794,0.00010180143,0.0002704683,0.0009794191,0.00001882521,0.00039394398,0.000004342137],"about_ca_topic_score_codex":0.01229661,"about_ca_topic_score_gemma":0.040923826,"teacher_disagreement_score":0.01229661,"about_ca_system_score_codex":0.0004767662,"about_ca_system_score_gemma":0.00027834764,"threshold_uncertainty_score":0.024450064},"labels":[],"label_agreement":null},{"id":"W2043962326","doi":"10.1088/0004-637x/696/1/1021","title":"THE SATURATION LIMIT OF THE MAGNETOROTATIONAL INSTABILITY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Dynamo; Magnetorotational instability; Magnetic field; Solar dynamo; Magnetic energy; Magnetohydrodynamics; Magnetic Prandtl number; Magnetic pressure","score_opus":0.007972198718946694,"score_gpt":0.2266840675349049,"score_spread":0.2187118688159582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043962326","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9125235,0.00075326697,0.036122695,0.00061017164,0.000024381376,0.000051474835,0.00016663331,0.0005152594,0.049232606],"genre_scores_gemma":[0.99665534,0.000117420335,0.001703367,0.000063018335,0.000011979958,0.000032297896,0.00006734644,0.000033313416,0.0013157749],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998418,0.000027706566,0.0000075984726,0.000030261685,0.000045390578,0.000047167687],"domain_scores_gemma":[0.99937195,0.00024164729,0.0000950105,0.000064731255,0.00012383956,0.00010281906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003083472,0.00021616448,0.00022033161,0.00030775834,0.00035886985,0.00081701716,0.00042112826,0.00048814112,0.0017990121],"category_scores_gemma":[0.002719619,0.0002218623,0.00026658791,0.00013220639,0.00089014444,0.0012207051,0.001090715,0.0006045195,0.00035272987],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013477412,0.0003250817,0.036491614,0.00069108664,0.00013800329,0.0015021001,0.002580392,0.27196553,0.32879066,0.3007901,0.004937436,0.05044028],"study_design_scores_gemma":[0.00011617026,0.00028057885,0.010596476,0.00009690933,0.000029155794,0.00048228426,0.00029934844,0.89357066,0.04198027,0.04840195,0.004099019,0.000047166144],"about_ca_topic_score_codex":0.0020334744,"about_ca_topic_score_gemma":0.0006842799,"teacher_disagreement_score":0.0020334744,"about_ca_system_score_codex":0.0004483547,"about_ca_system_score_gemma":0.00058819656,"threshold_uncertainty_score":0.0060183406},"labels":[],"label_agreement":null},{"id":"W2043978583","doi":"10.1088/0004-637x/791/2/78","title":"UNIVERSALITY OF THE ACCELERATION DUE TO GRAVITY ON THE SURFACE OF A RAPIDLY ROTATING NEUTRON STAR","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Gravitational acceleration; Angular velocity; Gravitation; Equator; Acceleration; Quadrupole; Flattening","score_opus":0.015356983421830403,"score_gpt":0.2908350442131865,"score_spread":0.2754780607913561,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043978583","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97730917,0.00028628088,0.010540145,0.00012244764,0.000032391228,0.000018831233,0.00006232911,0.0002961223,0.011332232],"genre_scores_gemma":[0.9981627,0.00013255373,0.001131026,0.0000126368805,0.000009212985,0.000005358278,0.00004645066,0.00006184806,0.0004382171],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.999843,0.000021372955,0.00000747503,0.000027066788,0.000054225835,0.000046760753],"domain_scores_gemma":[0.99971706,0.00006927042,0.00006646758,0.000045589666,0.0000540034,0.000047583762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026464098,0.00041662809,0.00038818503,0.0004817372,0.00031864143,0.0007323983,0.00039183925,0.0004489113,0.0008631957],"category_scores_gemma":[0.001695582,0.00028978844,0.0005757512,0.00040454298,0.0010380538,0.00051747466,0.0005230752,0.000497146,0.00022429871],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032547765,0.00007480755,0.053755805,0.00014114604,0.00010468665,0.001112248,0.00048627812,0.7866735,0.076300934,0.06371201,0.0007386128,0.016574554],"study_design_scores_gemma":[0.00008600907,0.00016837,0.08712106,0.00003552398,0.000059674887,0.00039634228,0.00009341932,0.88286024,0.011354049,0.015708422,0.0020276348,0.000089340574],"about_ca_topic_score_codex":0.0036143523,"about_ca_topic_score_gemma":0.0018562682,"teacher_disagreement_score":0.0036143523,"about_ca_system_score_codex":0.00063801795,"about_ca_system_score_gemma":0.0004430501,"threshold_uncertainty_score":0.007186651},"labels":[],"label_agreement":null},{"id":"W2043993903","doi":"10.1088/0004-637x/770/2/128","title":"SUPER-LUMINOUS TYPE Ic SUPERNOVAE: CATCHING A MAGNETAR BY THE TAIL","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":409,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Vetenskapsrådet; Queen's University; Danmarks Grundforskningsfond; U.S. Department of Energy; European Commission; Office of Science; Johns Hopkins University; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Smithsonian Institution; Durham University; Alfred P. Sloan Foundation; Queen's University Belfast; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Magnetar; Supernova; Luminosity; Ejecta; Galaxy; Redshift; Light curve; Astronomy; Neutron star","score_opus":0.008881567455005214,"score_gpt":0.21105313895609834,"score_spread":0.20217157150109313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2043993903","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983941,0.000070817856,0.00056855264,0.0000068781314,0.000001610061,0.000002222891,0.0002172657,0.00001937109,0.00071914936],"genre_scores_gemma":[0.9988747,0.000053265736,0.00035625667,0.000009287348,0.000003218572,0.0000013039275,0.00051054585,0.000005306609,0.00018605634],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999188,0.00000761313,0.000006684576,0.00002649768,0.000019723975,0.000020696547],"domain_scores_gemma":[0.9994549,0.00008369668,0.00025981426,0.000057291043,0.00004043341,0.00010390198],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020506437,0.00026613384,0.00016999409,0.00050354627,0.00020725038,0.00041439608,0.00027200597,0.00015867132,0.00094630494],"category_scores_gemma":[0.0005584767,0.00012367564,0.00024522588,0.00028635075,0.00021439472,0.00023803211,0.00035477913,0.00015773137,0.00027677283],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011994744,0.000014460553,0.9776858,0.000022698867,0.000039064278,0.0002555467,0.00004103102,0.0007113211,0.014954104,0.00020184931,0.00009879687,0.005855221],"study_design_scores_gemma":[0.000005379768,0.000103962775,0.98939145,0.0000075041817,0.000030297886,0.0012459992,0.00006195587,0.0020749767,0.005772827,0.00030333723,0.000994832,0.000007467808],"about_ca_topic_score_codex":0.0028653136,"about_ca_topic_score_gemma":0.007906929,"teacher_disagreement_score":0.0028653136,"about_ca_system_score_codex":0.00021622797,"about_ca_system_score_gemma":0.000100752426,"threshold_uncertainty_score":0.0056972504},"labels":[],"label_agreement":null},{"id":"W2044064672","doi":"10.1086/308734","title":"Prolate Cores in Filamentary Molecular Clouds","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Prolate spheroid; Molecular cloud; Astrobiology; Astronomy; Environmental science; Astrophysics; Geology; Physics; Classical mechanics","score_opus":0.005998803386904151,"score_gpt":0.22691924963332682,"score_spread":0.22092044624642268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044064672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97617733,0.00029351315,0.015389134,0.00021211784,0.000017509554,0.000020993919,0.000059755086,0.00004907165,0.00778067],"genre_scores_gemma":[0.99774265,0.00012120466,0.0013759703,0.00001996604,0.00001576965,0.000009929815,0.000024862242,0.000006524247,0.0006831249],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999547,0.00001020332,0.0000016067521,0.0000062805875,0.000009958864,0.00001727324],"domain_scores_gemma":[0.99984014,0.000029406427,0.000062532294,0.000014999622,0.000011755555,0.000041090752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000102394224,0.00022050457,0.00017456648,0.00022747455,0.00041703897,0.000743605,0.0004380097,0.0003715092,0.00073371513],"category_scores_gemma":[0.0005486753,0.00015731501,0.0002246283,0.00015646739,0.0006469258,0.0005927498,0.00051633676,0.00023172375,0.00013374278],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004531052,0.00010787063,0.028940728,0.00006761041,0.00006244002,0.0017603195,0.0005711959,0.7897422,0.02464341,0.14379063,0.0012276763,0.008632824],"study_design_scores_gemma":[0.00011229888,0.000109611625,0.009623661,0.000017110142,0.000020632393,0.00043407135,0.00011636172,0.9347931,0.0016360637,0.050107263,0.0030062415,0.000023632156],"about_ca_topic_score_codex":0.004580186,"about_ca_topic_score_gemma":0.0023774959,"teacher_disagreement_score":0.004580186,"about_ca_system_score_codex":0.00067931693,"about_ca_system_score_gemma":0.00020701793,"threshold_uncertainty_score":0.009107053},"labels":[],"label_agreement":null},{"id":"W2044066699","doi":"10.1088/0004-637x/723/1/563","title":"NUMERICAL SIMULATIONS OF THERMOHALINE CONVECTION: IMPLICATIONS FOR EXTRA-MIXING IN LOW-MASS RGB STARS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Convection; Stars; Radiative transfer; RGB color model; Stability (learning theory); Computer simulation","score_opus":0.014310417246340272,"score_gpt":0.278554135003334,"score_spread":0.26424371775699373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044066699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.976304,0.0003332067,0.012070048,0.0008308948,0.00009031246,0.000054935947,0.000498137,0.00025179915,0.009566707],"genre_scores_gemma":[0.9925781,0.00011868289,0.006177771,0.00008996695,0.000015927308,0.0000373175,0.00019611928,0.000046313664,0.0007397417],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998611,0.000042604173,0.000011505996,0.000018920675,0.000030990584,0.000034775363],"domain_scores_gemma":[0.9984457,0.00087247026,0.00022330882,0.00010229421,0.00016519772,0.0001910506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005689659,0.0005209109,0.00070299197,0.0004166871,0.00068424013,0.0011356053,0.00079692923,0.0012095597,0.001761396],"category_scores_gemma":[0.003125037,0.00040183254,0.00059967383,0.0004694374,0.0011077125,0.00074842264,0.00079172873,0.0007748355,0.00015798575],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014386694,0.00008384885,0.006571221,0.00004684219,0.000035204706,0.00010299195,0.000100680045,0.9859687,0.0027715468,0.0024612253,0.00023504377,0.0014787673],"study_design_scores_gemma":[0.000023668432,0.000013857131,0.0006245871,0.000005106074,0.0000050603016,0.000006433204,0.00001793205,0.99833614,0.0003663834,0.00049352634,0.00010275815,0.000004622104],"about_ca_topic_score_codex":0.014118664,"about_ca_topic_score_gemma":0.006393792,"teacher_disagreement_score":0.014118664,"about_ca_system_score_codex":0.0007860332,"about_ca_system_score_gemma":0.0007181588,"threshold_uncertainty_score":0.028073013},"labels":[],"label_agreement":null},{"id":"W2044114628","doi":"10.1088/0004-637x/743/2/183","title":"THE X-RAY COUNTERPART OF THE HIGH-<i>B</i>PULSAR PSR J0726–2612","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Pulsar; Neutron star; Millisecond pulsar; Observatory; RADIUS; Magnetic field; Pulsar planet; Stars","score_opus":0.013690947604006113,"score_gpt":0.2782823890085005,"score_spread":0.26459144140449437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044114628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965533,0.00010324967,0.0001875117,0.000038917093,0.000012243997,0.000007989226,0.00030788992,0.000041658517,0.002747224],"genre_scores_gemma":[0.996581,0.0001011904,0.00067388156,0.000073410556,0.000020723228,0.000011576951,0.0011422555,0.000013399842,0.0013826506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999368,0.000004113541,0.0000041094627,0.000024207699,0.000012287887,0.000018563378],"domain_scores_gemma":[0.9996488,0.000013232202,0.00018896707,0.000025412262,0.000027579592,0.00009598997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008390118,0.00034092367,0.00022525198,0.00050840096,0.00043464586,0.0004093524,0.0002453033,0.00029414246,0.0022117957],"category_scores_gemma":[0.00018324581,0.00013409881,0.00014394108,0.0006279085,0.00035534275,0.00019664485,0.0003499977,0.00029039555,0.0008787468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040548964,0.00019555441,0.539078,0.00015490636,0.00006741411,0.002587231,0.00031478144,0.0004850207,0.43724886,0.00094002334,0.0031346558,0.015388201],"study_design_scores_gemma":[0.00002989282,0.0002317101,0.97442734,0.000013315175,0.000020718102,0.0027006327,0.0002617469,0.00036898893,0.013825254,0.00016239143,0.007947671,0.000010296169],"about_ca_topic_score_codex":0.0009310827,"about_ca_topic_score_gemma":0.0020803348,"teacher_disagreement_score":0.0022117957,"about_ca_system_score_codex":0.00018114949,"about_ca_system_score_gemma":0.000111355694,"threshold_uncertainty_score":0.007399261},"labels":[],"label_agreement":null},{"id":"W2044186637","doi":"10.1086/529069","title":"Could the Ultra–Metal‐Poor Stars be Chemically Peculiar and Not Related to the First Stars?","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Stars; Physics; Astrophysics; T Tauri star; K-type main-sequence star; Abundance (ecology); Astronomy; Stellar collision; Galaxy","score_opus":0.012241276963070643,"score_gpt":0.21578093895449554,"score_spread":0.2035396619914249,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044186637","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925264,0.0024844378,0.00086347794,0.00076938275,0.00013775288,0.000012696582,0.0002188001,0.000020946225,0.0029660834],"genre_scores_gemma":[0.9962836,0.00084786065,0.00073652767,0.0007506402,0.00011416651,0.000007902493,0.00022961713,0.000011883904,0.0010177734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970835,0.000025087196,0.000020858917,0.00012028047,0.00004479883,0.00008054713],"domain_scores_gemma":[0.99856347,0.000108778026,0.000712325,0.0001943262,0.00017542219,0.00024566049],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067054824,0.00034252147,0.00069506286,0.00089840655,0.00077853474,0.0011234921,0.0005852414,0.00089966366,0.0018391608],"category_scores_gemma":[0.0016851344,0.00019135374,0.0003575195,0.00089718756,0.0015962344,0.0013537962,0.0007355227,0.0006519327,0.0007559792],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065712613,0.000068402114,0.94794583,0.0002049403,0.00020425502,0.0012168492,0.00077731424,0.00018731825,0.013458161,0.004358028,0.00077600987,0.03014575],"study_design_scores_gemma":[0.000026714672,0.00025088346,0.9741805,0.00006096747,0.00007678377,0.004903988,0.0010783429,0.00026116005,0.002148288,0.005550961,0.011433724,0.000027590562],"about_ca_topic_score_codex":0.0018140269,"about_ca_topic_score_gemma":0.002074475,"teacher_disagreement_score":0.0018391608,"about_ca_system_score_codex":0.00039943692,"about_ca_system_score_gemma":0.00026339348,"threshold_uncertainty_score":0.00615263},"labels":[],"label_agreement":null},{"id":"W2044194531","doi":"10.1086/318348","title":"On the Timescale for the Formation of Protostellar Cores in Magnetic Interstellar Clouds","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Physics; Molecular cloud; Astrophysics; Diffusion; Star formation; Interstellar medium; Interstellar cloud; Gravitational collapse; Flux (metallurgy); Plasma; Stars; Thermodynamics; Chemistry; Nuclear physics","score_opus":0.013720551907400345,"score_gpt":0.23847497693648273,"score_spread":0.22475442502908238,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044194531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9048343,0.006535668,0.060045682,0.00403656,0.0004495966,0.00008411948,0.0005369907,0.0004390906,0.023038024],"genre_scores_gemma":[0.9928745,0.0014100673,0.0039867084,0.000105981104,0.00013572743,0.00004412859,0.00014750633,0.00006741434,0.0012280318],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991786,0.0000089259565,0.000005204891,0.000029324694,0.000014946283,0.000023758506],"domain_scores_gemma":[0.99871457,0.0006316122,0.00030183568,0.00008371752,0.00008641224,0.00018188849],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008338033,0.00036071468,0.00035533443,0.00039072882,0.0009092102,0.0010568413,0.00082045415,0.00072685245,0.0026375228],"category_scores_gemma":[0.0057540783,0.00028909332,0.0004974007,0.00019129792,0.0005111802,0.0020585468,0.0008769492,0.0011912237,0.00030440747],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005356809,0.00017555284,0.09179032,0.00071351725,0.00013218076,0.00195909,0.0012050717,0.17476773,0.07901822,0.5846092,0.00587087,0.059222605],"study_design_scores_gemma":[0.00016548554,0.0002162556,0.06639283,0.000220104,0.0001513402,0.0010830438,0.0005220323,0.63280094,0.008850394,0.27855986,0.010919542,0.00011814792],"about_ca_topic_score_codex":0.0031636923,"about_ca_topic_score_gemma":0.0026569674,"teacher_disagreement_score":0.0031636923,"about_ca_system_score_codex":0.001835901,"about_ca_system_score_gemma":0.0006465301,"threshold_uncertainty_score":0.013320446},"labels":[],"label_agreement":null},{"id":"W2044316419","doi":"10.1086/501418","title":"First Attempt at Spectroscopic Detection of Gravity Modes in the Long‐Period Pulsating Subdwarf B Star PG 1627+017","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Subdwarf; Astrophysics; Balmer series; Radial velocity; Amplitude; Orbital motion; Stars; Astronomy; Orbital period; Spectral line; White dwarf; Emission spectrum; Optics; Angular momentum","score_opus":0.008868502295380786,"score_gpt":0.21940117529164607,"score_spread":0.2105326729962653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044316419","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970867,0.000099331475,0.0010710494,0.0000363782,0.000010617003,0.000016130525,0.00013902274,0.000042245112,0.0014985902],"genre_scores_gemma":[0.9944301,0.000081136306,0.003945391,0.000047115453,0.000022012424,0.000021197688,0.0008304222,0.000013341258,0.00060919847],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998989,0.000010965073,0.0000047144904,0.00002978675,0.000032158572,0.00002340398],"domain_scores_gemma":[0.9996655,0.000047583577,0.000063333086,0.000046525834,0.000055831424,0.000121282006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025348776,0.00024942556,0.00021871993,0.00061636884,0.0005067342,0.00038633146,0.00024103415,0.00034989446,0.0009498702],"category_scores_gemma":[0.00037415838,0.00018026555,0.00014919371,0.00043503963,0.00019437785,0.00017291318,0.00047925703,0.00032546002,0.00046237741],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003922415,0.00027750246,0.6676738,0.00008921545,0.00010167515,0.0009017163,0.000761956,0.0004172477,0.29098594,0.0005145597,0.0011057588,0.03677831],"study_design_scores_gemma":[0.000022106158,0.00048265292,0.9787931,0.00001014556,0.00003917885,0.00042832555,0.00022175595,0.001275008,0.015103907,0.00017915817,0.0034336473,0.0000109306775],"about_ca_topic_score_codex":0.0011214424,"about_ca_topic_score_gemma":0.003110723,"teacher_disagreement_score":0.0011214424,"about_ca_system_score_codex":0.00017256005,"about_ca_system_score_gemma":0.00019408969,"threshold_uncertainty_score":0.0031775832},"labels":[],"label_agreement":null},{"id":"W2044371148","doi":"10.1086/522956","title":"The Globular Cluster System of M60 (NGC 4649). I. Canada‐France‐Hawaii Telescope MOS Spectroscopy and Database","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Velocity dispersion; Photometry (optics); Radial velocity; Virgo Cluster; Astronomy; Red-giant branch; Galaxy; Spectrograph; Elliptical galaxy; Stars; Spectral line","score_opus":0.004648776015319418,"score_gpt":0.18922395595074282,"score_spread":0.1845751799354234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044371148","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.038016118,0.00058471976,0.0005144367,0.00006551096,0.000016336668,0.00014706254,0.94411135,0.001069093,0.015475304],"genre_scores_gemma":[0.021280553,0.00038522793,0.0010954313,0.000043978696,0.000006866179,0.00008904773,0.9734963,0.00007542566,0.003527103],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99972624,0.000010001204,0.000025636626,0.00007631002,0.000101378384,0.00006043595],"domain_scores_gemma":[0.99920076,0.000032189026,0.00010899891,0.00013451408,0.0002550254,0.0002685566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003785515,0.00081370067,0.0003865121,0.00562659,0.0008331604,0.0007946009,0.0011634656,0.0003168242,0.022173658],"category_scores_gemma":[0.0010512277,0.00023786152,0.00026384942,0.0072522755,0.00018813615,0.00052410655,0.0010106104,0.00025948486,0.013411418],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000626633,0.00013922947,0.2043766,0.0014744947,0.00019091545,0.00035947442,0.00085825066,0.00087167596,0.0066154688,0.004193328,0.63004094,0.15025291],"study_design_scores_gemma":[0.000071336755,0.000027860287,0.38991532,0.00017503035,0.000060845618,0.00020934589,0.00022154202,0.00065328233,0.0017308783,0.00045323648,0.60644954,0.000031817024],"about_ca_topic_score_codex":0.49667427,"about_ca_topic_score_gemma":0.4504385,"teacher_disagreement_score":0.49667427,"about_ca_system_score_codex":0.0017717438,"about_ca_system_score_gemma":0.0039501414,"threshold_uncertainty_score":0.9875666},"labels":[],"label_agreement":null},{"id":"W2044531289","doi":"10.1086/510308","title":"Infrared Spectroscopy of the Ultra-Low-Mass Binary Oph 162225-240515","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Ophiuchus; Brown dwarf; Surface gravity; Astrophysics; Physics; Low Mass; Spectral line; Binary number; Spectroscopy; Star formation; Astronomy; Stars","score_opus":0.005427657500033431,"score_gpt":0.20695855338796115,"score_spread":0.20153089588792772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044531289","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99855274,0.00014652988,0.00009249786,0.000012458722,0.0000045451516,0.0000023092011,0.00009570219,0.000011885747,0.0010813632],"genre_scores_gemma":[0.99861574,0.000046503756,0.00027571685,0.000025282134,0.000006137222,0.0000026490027,0.00055232184,0.000003625125,0.00047192024],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993634,0.0000039353085,0.0000031486522,0.000022711238,0.000020165282,0.0000138072855],"domain_scores_gemma":[0.99991953,0.000006707282,0.00002507037,0.0000058916103,0.000011272063,0.00003150373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111882124,0.00018346189,0.00022698642,0.00037978677,0.00035415398,0.0003258966,0.00019689738,0.00032295426,0.001153959],"category_scores_gemma":[0.00018759859,0.00009641551,0.0000812804,0.0002512644,0.00011857815,0.0001787329,0.00034509605,0.00020222062,0.00034588887],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005602097,0.0003298983,0.36321864,0.00011541446,0.00008084036,0.0021275545,0.0004600927,0.000924016,0.61001617,0.00053351634,0.0012131421,0.020420482],"study_design_scores_gemma":[0.00002123367,0.0002214396,0.98563856,0.000009838047,0.000017590242,0.0006727296,0.0001564572,0.0014390426,0.010237315,0.000085761894,0.0014921658,0.0000077044],"about_ca_topic_score_codex":0.0011911483,"about_ca_topic_score_gemma":0.0017716417,"teacher_disagreement_score":0.0011911483,"about_ca_system_score_codex":0.00017246266,"about_ca_system_score_gemma":0.000065390326,"threshold_uncertainty_score":0.0038603544},"labels":[],"label_agreement":null},{"id":"W2044642016","doi":"10.1088/0004-637x/797/2/83","title":"THE FINAL FATE OF STARS THAT IGNITE NEON AND OXYGEN OFF-CENTER: ELECTRON CAPTURE OR IRON CORE-COLLAPSE SUPERNOVA?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Neon; Supernova; Stellar evolution; Electron capture; Stars; Convection; White dwarf; Chandrasekhar limit; Instability","score_opus":0.01513776686965503,"score_gpt":0.23159681579908234,"score_spread":0.2164590489294273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044642016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945491,0.0003950792,0.0014957538,0.00010363718,0.00001291438,0.000008087318,0.00005660622,0.000018702425,0.0033601497],"genre_scores_gemma":[0.997538,0.00022704384,0.00046300908,0.000035072415,0.0000060139546,0.0000031907175,0.00010232897,0.000009890573,0.0016155097],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999317,0.00000721747,0.0000038009966,0.000017818116,0.000012651106,0.000026816791],"domain_scores_gemma":[0.9998876,0.000010981232,0.000026126416,0.000015225545,0.000017158667,0.000042878568],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031201582,0.0001807754,0.00032704198,0.00017804757,0.0004943725,0.00080301426,0.00033531754,0.00046345653,0.00081217155],"category_scores_gemma":[0.0004255962,0.00010683794,0.00024100863,0.00007916069,0.0003894572,0.0006295249,0.00043418453,0.00035119042,0.00027353122],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023088164,0.00037384973,0.43946505,0.00023721537,0.00015107237,0.004640115,0.0014862975,0.0114859035,0.38444868,0.09429033,0.0014480115,0.05966471],"study_design_scores_gemma":[0.00013416582,0.0015505144,0.6232113,0.00024699167,0.00013811007,0.006936602,0.004202089,0.066233955,0.19175546,0.08576047,0.019690672,0.00013969143],"about_ca_topic_score_codex":0.0012419831,"about_ca_topic_score_gemma":0.0012386339,"teacher_disagreement_score":0.0012419831,"about_ca_system_score_codex":0.00041343176,"about_ca_system_score_gemma":0.0001722674,"threshold_uncertainty_score":0.0029996634},"labels":[],"label_agreement":null},{"id":"W2044726038","doi":"10.1088/0004-637x/764/1/38","title":"DISCOVERY OF TeV GAMMA-RAY EMISSION FROM CTA 1 BY VERITAS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Fermi Gamma-ray Space Telescope; Supernova remnant; Pulsar wind nebula; Supernova; Binary pulsar; Nebula; Crab Nebula; Photon","score_opus":0.00511943773613505,"score_gpt":0.19973281747564534,"score_spread":0.1946133797395103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044726038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952479,0.0002639251,0.00065365277,0.000053776803,0.000015474785,0.000012159615,0.0006488271,0.00009691685,0.0030074911],"genre_scores_gemma":[0.99527514,0.00021084362,0.0020815774,0.000055385357,0.000016871132,0.0000074297755,0.0015095255,0.000025491152,0.00081784645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998497,0.000007827423,0.0000050987624,0.000042742216,0.000065015236,0.000029690418],"domain_scores_gemma":[0.9994615,0.00008252617,0.00023198403,0.000060617556,0.00006241789,0.000101010046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002262285,0.00022914985,0.0001861521,0.0009670753,0.0003686601,0.0009413837,0.00050556957,0.00035270784,0.0014327379],"category_scores_gemma":[0.00092185294,0.00023221145,0.00021281793,0.0006370285,0.00029174922,0.00030633155,0.0007742381,0.0006051801,0.00034253518],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074886123,0.00008381834,0.63468605,0.00013494332,0.0001101868,0.0074883588,0.0009874938,0.0011314894,0.3059228,0.0022050056,0.001652453,0.044848584],"study_design_scores_gemma":[0.0000580135,0.0004583219,0.9273566,0.00007218114,0.000099590114,0.012379336,0.00030076536,0.0042890403,0.03380208,0.00080318144,0.020336354,0.000044522723],"about_ca_topic_score_codex":0.005008019,"about_ca_topic_score_gemma":0.010371049,"teacher_disagreement_score":0.005008019,"about_ca_system_score_codex":0.00043382708,"about_ca_system_score_gemma":0.0002931296,"threshold_uncertainty_score":0.009957731},"labels":[],"label_agreement":null},{"id":"W2044739223","doi":"10.1086/586889","title":"C<sub>2</sub>in Peculiar DQ White Dwarfs","year":2008,"lang":"fr","type":"article","venue":"The Astrophysical Journal","topic":"Protein Degradation and Inhibitors","field":"Biochemistry, Genetics and Molecular Biology","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"White dwarf; White (mutation); Astrophysics; Physics; Astronomy; Stars; Biology; Genetics","score_opus":0.008383683940635288,"score_gpt":0.21415029542164193,"score_spread":0.20576661148100664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044739223","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99838066,0.00019361882,0.00014513679,0.000018206549,0.0000060312223,0.0000024749465,0.00009121603,0.000011769267,0.0011508649],"genre_scores_gemma":[0.9992638,0.00005607195,0.000093703085,0.000023165243,0.000010543939,0.0000015365772,0.00016387133,0.0000064279106,0.00038077994],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99991393,0.000004911132,0.000005721662,0.000036625916,0.000015779508,0.000023042405],"domain_scores_gemma":[0.999795,0.00001340437,0.000086363194,0.0000143755515,0.000026403999,0.00006439125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010850531,0.00019322275,0.0002462446,0.00066987984,0.00050541107,0.0005921597,0.00020844121,0.00029460806,0.0012852884],"category_scores_gemma":[0.0002982981,0.00012344083,0.000120858516,0.0005480144,0.00045907416,0.00022742533,0.00040121435,0.00016020052,0.00025805907],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005897999,0.00007336402,0.8485271,0.0000586976,0.000053262054,0.0019325279,0.00047478924,0.0003119498,0.13688867,0.0014272402,0.00058588764,0.009076716],"study_design_scores_gemma":[0.000009024621,0.00006130922,0.98951435,0.0000057025045,0.000017184277,0.0022873005,0.00031217988,0.00046466338,0.004147953,0.0007582322,0.0024160552,0.0000060331513],"about_ca_topic_score_codex":0.0058486187,"about_ca_topic_score_gemma":0.0049328054,"teacher_disagreement_score":0.0058486187,"about_ca_system_score_codex":0.00045906077,"about_ca_system_score_gemma":0.00013685053,"threshold_uncertainty_score":0.011629164},"labels":[],"label_agreement":null},{"id":"W2044771473","doi":"10.1086/527473","title":"Spiral Inflow Feeding the Nuclear Starburst in M83, Observed in Hα Emission with the GHαFaS Fabry-Perot Interferometer","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Galaxy; Spiral galaxy; RADIUS; Astronomy; Star formation; Interferometry","score_opus":0.016612968345029993,"score_gpt":0.20352884908695806,"score_spread":0.18691588074192808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044771473","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99933356,0.00004897245,0.00007037642,0.000016442278,0.000001434785,0.000002062523,0.00013765952,0.000020284766,0.00036921338],"genre_scores_gemma":[0.9993205,0.00005425578,0.00024905658,0.000011686419,0.00000539072,0.0000027514363,0.00020154605,0.000003582128,0.00015129417],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999473,0.000004586764,0.0000030408419,0.00001378369,0.000009769413,0.000021494747],"domain_scores_gemma":[0.9998115,0.00001554002,0.000081211394,0.000022088467,0.000017802151,0.000051955023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009114515,0.00016622491,0.00022199455,0.00034167693,0.00040208944,0.00028841032,0.0002474746,0.0003116677,0.00049020373],"category_scores_gemma":[0.00026250875,0.0001533093,0.00013029968,0.00046632747,0.00020142952,0.0001660209,0.00025343845,0.00021118972,0.00027293572],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051612273,0.000137635,0.92264134,0.00005053309,0.00005672162,0.002777664,0.00093962456,0.0009295738,0.058667064,0.0002575739,0.0007686378,0.012257534],"study_design_scores_gemma":[0.000009363432,0.00004177596,0.99709606,0.0000041314165,0.000014637732,0.0005240862,0.00008036056,0.0007802887,0.0010469275,0.000042816802,0.00035595245,0.0000035948187],"about_ca_topic_score_codex":0.009441943,"about_ca_topic_score_gemma":0.017977588,"teacher_disagreement_score":0.009441943,"about_ca_system_score_codex":0.00031767774,"about_ca_system_score_gemma":0.00014226206,"threshold_uncertainty_score":0.018773973},"labels":[],"label_agreement":null},{"id":"W2044807635","doi":"10.1088/0004-637x/705/1/1000","title":"EFFECTS OF FOSSIL MAGNETIC FIELDS ON CONVECTIVE CORE DYNAMOS IN A-TYPE STARS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Dynamo; Physics; Convection; Dynamo theory; Magnetic field; Solar dynamo; Equipartition theorem; Magnetohydrodynamics; Astrophysics; Radiative transfer; Differential rotation; Magnetic energy; Mercury's magnetic field; Classical mechanics; Mechanics; L-shell; Computational physics; Stars; Earth's magnetic field","score_opus":0.005457402113750702,"score_gpt":0.225034636123545,"score_spread":0.2195772340097943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044807635","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99713564,0.000046488887,0.000714923,0.000067677895,0.000009516788,0.000007093574,0.00005347568,0.000035106248,0.0019301652],"genre_scores_gemma":[0.99933213,0.000028883787,0.00042385966,0.000018970308,0.0000029478267,0.000004675382,0.00003144981,0.000014065816,0.00014293543],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992406,0.00002067541,0.000005515838,0.000010248354,0.000012997059,0.000026497668],"domain_scores_gemma":[0.99946815,0.00023624183,0.00008795804,0.000031263262,0.000044459703,0.00013195834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034848944,0.0003547203,0.00035146187,0.00025724768,0.0005408636,0.000820952,0.000384161,0.0005732294,0.00079653144],"category_scores_gemma":[0.001377215,0.00023976184,0.0004190447,0.0002355734,0.00075639534,0.00036975174,0.0006821901,0.0005131862,0.00009940947],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033215966,0.00017404734,0.022120822,0.00004410109,0.000052027157,0.00027913792,0.00013299874,0.957914,0.014004943,0.00222984,0.00021891532,0.0024970202],"study_design_scores_gemma":[0.00006811569,0.00014514365,0.0073221317,0.000012551825,0.000016850121,0.000033920456,0.00009818926,0.98902214,0.0024541756,0.00055628904,0.00025570573,0.000014782995],"about_ca_topic_score_codex":0.011438029,"about_ca_topic_score_gemma":0.005975788,"teacher_disagreement_score":0.011438029,"about_ca_system_score_codex":0.0007405476,"about_ca_system_score_gemma":0.0007550814,"threshold_uncertainty_score":0.022742927},"labels":[],"label_agreement":null},{"id":"W2044850206","doi":"10.1088/0004-637x/710/2/1672","title":"THE ACS FORNAX CLUSTER SURVEY. IX. THE COLOR-MAGNITUDE RELATION OF GLOBULAR CLUSTER SYSTEMS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Fornax Cluster; Virgo Cluster; Galaxy; Cluster (spacecraft); Galaxy cluster; Star cluster","score_opus":0.007568930535027145,"score_gpt":0.21629111966823894,"score_spread":0.2087221891332118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044850206","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6045415,0.001355606,0.0008405866,0.0011568797,0.00010709474,0.0001849219,0.34034616,0.0011871923,0.050280035],"genre_scores_gemma":[0.65304697,0.00090380776,0.0045818193,0.0005201524,0.00014894942,0.00023665531,0.31926113,0.00021909164,0.021081515],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980193,0.000015043372,0.000010660575,0.000056857727,0.000070343965,0.00004526911],"domain_scores_gemma":[0.9993782,0.000035710123,0.00021761058,0.00008014833,0.00016224508,0.00012594117],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003172253,0.00036437446,0.00026425574,0.0024799658,0.0003530424,0.0006501553,0.00042381647,0.0002698558,0.0084697995],"category_scores_gemma":[0.00087932544,0.00011900577,0.00025967593,0.002600787,0.00012816036,0.0004315299,0.0007736219,0.000297712,0.0049630147],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016210068,0.000053486237,0.84024596,0.0001557947,0.00013381401,0.0001124549,0.00042746981,0.00031129963,0.0028329429,0.0015666556,0.113669835,0.040328212],"study_design_scores_gemma":[0.000010548015,0.0000111969175,0.9741538,0.000011952339,0.000011332923,0.00004666522,0.000095985415,0.00017502338,0.00015922752,0.00012467483,0.02519591,0.0000036348436],"about_ca_topic_score_codex":0.044195294,"about_ca_topic_score_gemma":0.056473743,"teacher_disagreement_score":0.044195294,"about_ca_system_score_codex":0.0005399514,"about_ca_system_score_gemma":0.0003426358,"threshold_uncertainty_score":0.08787608},"labels":[],"label_agreement":null},{"id":"W2044867738","doi":"10.1086/507262","title":"<i>Chandra</i>Observations of the Transient 7 s X‐ray Pulsar AX J1845.0−0258","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Research Canada; McGill University","funders":"","keywords":"Pulsar; Black-body radiation; Neutron star; Observatory; Power law; Flux (metallurgy); Transient (computer programming)","score_opus":0.011994916809843775,"score_gpt":0.2101076436154802,"score_spread":0.19811272680563644,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2044867738","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9920204,0.0002197615,0.0003423738,0.00006818842,0.000016719088,0.000013478581,0.0025880456,0.00017964262,0.004551371],"genre_scores_gemma":[0.98713964,0.00022095582,0.0031239449,0.000076329416,0.000041536245,0.00001308071,0.008141851,0.000025147065,0.001217428],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999404,0.0000033338301,0.0000052554506,0.000010905874,0.000020157462,0.000019962103],"domain_scores_gemma":[0.99980456,0.000015455787,0.000069197915,0.000027091573,0.000023002143,0.00006065809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010774183,0.00016399927,0.00014973928,0.0012262056,0.0003648258,0.00033774378,0.00024443105,0.00018106091,0.002391582],"category_scores_gemma":[0.00022773758,0.00010941548,0.00013638001,0.00063554855,0.00013867117,0.00020519033,0.00037577213,0.00020274807,0.00033512994],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016731035,0.000489772,0.63370556,0.00042585298,0.00025839295,0.0042121494,0.00058644207,0.0023054285,0.24677752,0.0016109981,0.021922138,0.08603266],"study_design_scores_gemma":[0.000038659284,0.00012292633,0.9849539,0.000015324398,0.000034248525,0.0010623261,0.00007343018,0.00068390794,0.0046432945,0.00011476301,0.008245024,0.000012252926],"about_ca_topic_score_codex":0.004156147,"about_ca_topic_score_gemma":0.014778574,"teacher_disagreement_score":0.004156147,"about_ca_system_score_codex":0.00017353901,"about_ca_system_score_gemma":0.0001385723,"threshold_uncertainty_score":0.008263886},"labels":[],"label_agreement":null},{"id":"W2045196799","doi":"10.1086/422680","title":"Carbon‐Chain Oxides in Proton‐Irradiated CO Ice Films","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Interstellar ice; Carbon fibers; Cosmic ray; Interstellar medium; Cosmic dust; Astrochemistry; Spectral line; Irradiation; Absorption (acoustics); Proton; Interstellar cloud; Astrophysics; Astrobiology; Cosmochemistry; Molecule; Carbon chain; Astronomy; Materials science; Chemistry; Optics; Galaxy; Nuclear physics; Composite material","score_opus":0.00942054822391931,"score_gpt":0.24150062015603316,"score_spread":0.23208007193211386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045196799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978173,0.00037000483,0.00010816224,0.000011511511,0.000007448731,0.0000034298214,0.00009493374,0.000007424122,0.0015798152],"genre_scores_gemma":[0.9978701,0.00032529666,0.00018267373,0.000019684108,0.000006851045,0.000006331361,0.0002815017,0.0000120492,0.0012954557],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999505,0.0000032646765,0.0000015638951,0.000013145296,0.00001612907,0.000015408472],"domain_scores_gemma":[0.99988747,0.000029232442,0.000029158045,0.000005742348,0.000029681123,0.000018660365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000050202478,0.00021258493,0.0000999652,0.00031850688,0.00025616732,0.00021461582,0.00016735343,0.00018316107,0.0015051349],"category_scores_gemma":[0.0001220273,0.00010927055,0.0000898525,0.00022328987,0.00018540208,0.00017666425,0.00010802381,0.0002974816,0.00012622698],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012019193,0.000017654176,0.0006689184,0.000035191817,0.00000865916,0.00012083323,0.000050643608,0.00009168283,0.99792695,0.00003391249,0.00004647208,0.00087886886],"study_design_scores_gemma":[0.000011060659,0.00023120745,0.036409628,0.000015137142,0.000028465034,0.0002074567,0.00017191024,0.0008504458,0.9608922,0.000036395046,0.001139808,0.0000062282875],"about_ca_topic_score_codex":0.0013461385,"about_ca_topic_score_gemma":0.0008939527,"teacher_disagreement_score":0.0015051349,"about_ca_system_score_codex":0.00015456826,"about_ca_system_score_gemma":0.000056563484,"threshold_uncertainty_score":0.005035162},"labels":[],"label_agreement":null},{"id":"W2045218264","doi":"10.1088/0004-637x/783/2/95","title":"SYSTEMATIC PROBLEMS WITH USING DARK MATTER SIMULATIONS TO MODEL STELLAR HALOS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Dark matter; Halo; Dark matter halo; Cuspy halo problem; Scalar field dark matter; Stellar mass; Baryon; Baryonic dark matter","score_opus":0.017221942062694423,"score_gpt":0.26443521787208735,"score_spread":0.24721327580939292,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045218264","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":"methods","model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":"methods","domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7613413,0.00199736,0.20963275,0.0041064615,0.00057586585,0.0005034075,0.0015906446,0.0052304883,0.015021801],"genre_scores_gemma":[0.9250998,0.000682206,0.06940799,0.000859536,0.000095596944,0.00038007944,0.00078578136,0.0015382397,0.0011507492],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9936778,0.003884129,0.0005339226,0.000582321,0.0010912076,0.00023062619],"domain_scores_gemma":[0.946488,0.031569462,0.0033687837,0.012842763,0.0047425213,0.0009884743],"candidate_categories":["metaresearch"],"consensus_categories":[],"category_scores_codex":[0.014225073,0.0014634995,0.0010894233,0.0010138617,0.0020523486,0.0025342372,0.0035341275,0.0010744863,0.0011721428],"category_scores_gemma":[0.062240772,0.0013390139,0.0014278792,0.0016259251,0.0019093462,0.003167969,0.002700466,0.0023394611,0.00056050584],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049329875,0.00023202795,0.048004583,0.00039939297,0.0007656393,0.00022914549,0.0011947005,0.8869465,0.0067130933,0.031758577,0.0031723266,0.020090623],"study_design_scores_gemma":[0.0002104044,0.00018009802,0.006347073,0.00014294942,0.00014272166,0.00010519882,0.00025494842,0.9459625,0.008198295,0.033257015,0.005085565,0.00011318404],"about_ca_topic_score_codex":0.027255576,"about_ca_topic_score_gemma":0.023642242,"teacher_disagreement_score":0.98577493,"about_ca_system_score_codex":0.002401387,"about_ca_system_score_gemma":0.0023350525,"threshold_uncertainty_score":0.0752303},"labels":[],"label_agreement":null},{"id":"W2045292858","doi":"10.1086/375336","title":"On the Relationship between Cooling Flows and Bubbles","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Victoria","funders":"","keywords":"Cooling flow; Intracluster medium; Surface brightness; Cluster (spacecraft); Flow (mathematics); Galaxy cluster; Range (aeronautics)","score_opus":0.03804145347716133,"score_gpt":0.29005817187354815,"score_spread":0.25201671839638684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045292858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96533173,0.004254742,0.01358353,0.0022015856,0.00010334631,0.000035601337,0.000115699564,0.00009957997,0.014274182],"genre_scores_gemma":[0.9966354,0.0010758863,0.0011238251,0.00013265088,0.00012180382,0.000014061773,0.00006166769,0.00002198869,0.00081280764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963284,0.00013287054,0.000018207753,0.000071988754,0.000059112175,0.00008498129],"domain_scores_gemma":[0.9848274,0.011525321,0.0021621552,0.00044473138,0.0005247793,0.000515591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008850721,0.0002816047,0.00031858584,0.000647509,0.0007159833,0.0015291026,0.0006978259,0.00093184144,0.0031227905],"category_scores_gemma":[0.012636682,0.00034137102,0.00030870072,0.00053101644,0.0018664427,0.0025252937,0.00097762,0.0008310268,0.00023212378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016072617,0.00037746652,0.42393857,0.0007491178,0.00025346904,0.0037789498,0.0030580752,0.06455242,0.03608731,0.38538074,0.0078009423,0.07241568],"study_design_scores_gemma":[0.00025328837,0.00066959794,0.38634855,0.00029420183,0.0004263886,0.0048639365,0.001958463,0.25764656,0.017287409,0.3096418,0.020334613,0.00027524243],"about_ca_topic_score_codex":0.0028725103,"about_ca_topic_score_gemma":0.0011311651,"teacher_disagreement_score":0.0031227905,"about_ca_system_score_codex":0.0006088774,"about_ca_system_score_gemma":0.0002756949,"threshold_uncertainty_score":0.010446727},"labels":[],"label_agreement":null},{"id":"W2045322559","doi":"10.1088/0004-637x/722/2/1707","title":"ULTRA-COMPACT DWARFS IN THE CORE OF THE COMA CLUSTER","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McMaster University","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Physics; Astrophysics; Coma Cluster; Astronomy; Dwarf galaxy; Advanced Camera for Surveys; Galaxy cluster; Galaxy; Hubble space telescope","score_opus":0.008926437763255982,"score_gpt":0.22475194567914183,"score_spread":0.21582550791588584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045322559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994448,0.000043557196,0.00008565946,0.00000725163,7.022809e-7,0.0000011909696,0.0000544933,0.000007831824,0.0003545688],"genre_scores_gemma":[0.99958974,0.000021852862,0.00010373924,0.0000052108744,0.000001272148,6.664527e-7,0.00013759216,0.0000012471168,0.00013872249],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999915,0.000006428659,0.0000034436562,0.000018062889,0.000020111978,0.00003686759],"domain_scores_gemma":[0.99972814,0.000019557403,0.000094190305,0.000030483177,0.000044648776,0.000082980565],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011100837,0.00013692728,0.00014260785,0.0005884363,0.0004410328,0.0004030412,0.00017218874,0.00006647589,0.0010963754],"category_scores_gemma":[0.00037687385,0.00008490993,0.000081349724,0.0006441609,0.00023792955,0.00017810904,0.00045355392,0.00009979271,0.00022580914],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000095584044,0.000017594744,0.9762186,0.000011437954,0.000032283268,0.0002925388,0.00037342415,0.00019933589,0.015471185,0.0003177608,0.00026630014,0.006704072],"study_design_scores_gemma":[0.0000018051229,0.000022722117,0.99755716,0.0000022091806,0.000008691437,0.0002227986,0.00017285887,0.00025889865,0.00084758626,0.000072636125,0.00082975655,0.000002726169],"about_ca_topic_score_codex":0.01498062,"about_ca_topic_score_gemma":0.020086767,"teacher_disagreement_score":0.01498062,"about_ca_system_score_codex":0.00037177987,"about_ca_system_score_gemma":0.00020922693,"threshold_uncertainty_score":0.029786825},"labels":[],"label_agreement":null},{"id":"W2045405870","doi":"10.1086/322978","title":"X‐Ray Observations of the Supernova Remnant G21.5−0.9","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Physics; Astrophysics; Supernova remnant; Ionization; ROSAT; Line (geometry); Surface brightness; Calibration; Supernova; Astronomy; Galaxy","score_opus":0.019396039510551664,"score_gpt":0.22501779756665283,"score_spread":0.20562175805610117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045405870","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974286,0.00016376047,0.00011082743,0.000010969593,0.000003485184,0.000016662265,0.0010535793,0.000052114912,0.0011599954],"genre_scores_gemma":[0.9920237,0.0002451625,0.00079353974,0.00002515021,0.00001822479,0.000013586659,0.0059839203,0.000020949637,0.00087568443],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998771,0.000009956287,0.000011233918,0.000030902214,0.000036744284,0.0000341004],"domain_scores_gemma":[0.9996909,0.000018470175,0.00009032194,0.00005237752,0.000055793185,0.00009216031],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034255412,0.00046160762,0.0003070368,0.0013533656,0.00044770126,0.0004869256,0.0003467845,0.00028654002,0.0009479852],"category_scores_gemma":[0.00025715545,0.0001389739,0.0004351653,0.0007987817,0.00013964086,0.00017095833,0.00044921675,0.00024623427,0.00069619744],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014306082,0.0004808949,0.74441534,0.00020213777,0.00037493478,0.003235392,0.0010090882,0.0013510803,0.21084903,0.0003652146,0.0020150638,0.034271196],"study_design_scores_gemma":[0.000010662866,0.00020181538,0.99280155,0.0000046243513,0.00003682692,0.00066444156,0.00004820583,0.00024067427,0.0030000785,0.000023878276,0.0029582263,0.000009139797],"about_ca_topic_score_codex":0.0028577282,"about_ca_topic_score_gemma":0.0046598627,"teacher_disagreement_score":0.0028577282,"about_ca_system_score_codex":0.0002521908,"about_ca_system_score_gemma":0.00010183035,"threshold_uncertainty_score":0.00568223},"labels":[],"label_agreement":null},{"id":"W2045483442","doi":"10.1088/0004-637x/795/1/32","title":"STABILITY OF THE KEPLER-11 SYSTEM AND ITS ORIGIN","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Kepler; Astronomy; Astrobiology; Physics; Planet","score_opus":0.013814494881743385,"score_gpt":0.21735009660151683,"score_spread":0.20353560171977345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045483442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949817,0.00023537256,0.0014796564,0.000049072485,0.000006241699,0.0000039334304,0.00013161793,0.000028934854,0.0030834512],"genre_scores_gemma":[0.99888116,0.000047281723,0.0005237829,0.0000037576733,0.0000036490499,0.0000028089614,0.000109685105,0.000009297014,0.00041858695],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999075,0.000010904672,0.0000054756833,0.000041657302,0.000017026905,0.000017426231],"domain_scores_gemma":[0.99948835,0.00012541148,0.00015768185,0.000049972714,0.000099796234,0.00007881224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017866831,0.00016614047,0.00027183746,0.00059063046,0.00067018345,0.0008204358,0.00024205554,0.00036841293,0.0017302535],"category_scores_gemma":[0.001645137,0.00013306274,0.00015676486,0.00041463517,0.00048426408,0.00064115116,0.00060688466,0.00030901964,0.00041043322],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012163242,0.00012949908,0.641926,0.00029518438,0.00028170383,0.0013496494,0.00252922,0.1264598,0.12183104,0.03720804,0.0031320318,0.06364146],"study_design_scores_gemma":[0.00006515671,0.0005054114,0.6281516,0.00006730879,0.000113320835,0.0018196951,0.0013329944,0.30510038,0.027160741,0.024127487,0.011414549,0.00014127317],"about_ca_topic_score_codex":0.0016645566,"about_ca_topic_score_gemma":0.0007154918,"teacher_disagreement_score":0.0017302535,"about_ca_system_score_codex":0.00041780755,"about_ca_system_score_gemma":0.00018885364,"threshold_uncertainty_score":0.0057883263},"labels":[],"label_agreement":null},{"id":"W2045640061","doi":"10.1088/0004-637x/741/1/20","title":"CONSTRAINING TYPE Ia SUPERNOVAE PROGENITORS FROM THREE YEARS OF SUPERNOVA LEGACY SURVEY DATA","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Defence Research and Development Canada; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Supernova; Type (biology); Stars; Stellar evolution; Cosmology","score_opus":0.07633575988030986,"score_gpt":0.2774070604416154,"score_spread":0.20107130056130554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045640061","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9675404,0.0005329618,0.0020235248,0.00012907397,0.0000420127,0.000032589287,0.02466096,0.0002238201,0.004814736],"genre_scores_gemma":[0.9440182,0.0007533567,0.007270543,0.000059398895,0.000056551242,0.000043238393,0.044811998,0.00009416837,0.0028925503],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983,0.000017084074,0.00002849009,0.000052198997,0.000037590464,0.00003459071],"domain_scores_gemma":[0.9972258,0.0007674876,0.00061233883,0.0003657024,0.0005568423,0.0004717783],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012539595,0.0003032705,0.00026709266,0.004189757,0.0005849598,0.0015063708,0.0005976383,0.00042247304,0.002218006],"category_scores_gemma":[0.0020661908,0.00044248352,0.00056558906,0.0033446073,0.00015774973,0.0004751819,0.00081232795,0.00043645254,0.0011784896],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002742803,0.00006931407,0.958462,0.000063182604,0.00023759695,0.00021938865,0.0002387285,0.0023590056,0.0065292893,0.0004244951,0.0038906895,0.027232151],"study_design_scores_gemma":[0.000012499472,0.000031042768,0.99077916,0.000024866156,0.00008642098,0.00013642936,0.00017300168,0.0016442316,0.0013007896,0.00014980375,0.0056487517,0.000013027537],"about_ca_topic_score_codex":0.04586176,"about_ca_topic_score_gemma":0.11752596,"teacher_disagreement_score":0.04586176,"about_ca_system_score_codex":0.0004928283,"about_ca_system_score_gemma":0.00064572773,"threshold_uncertainty_score":0.09118962},"labels":[],"label_agreement":null},{"id":"W2045643973","doi":"10.1088/0004-637x/758/1/4","title":"ONE THOUSAND AND ONE CLUSTERS: MEASURING THE BULK FLOW WITH THE PLANCK ESZ AND X-RAY-SELECTED GALAXY CLUSTER CATALOGS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"CMB cold spot; ROSAT; Planck; Physics; Astrophysics; Galaxy cluster; Cluster (spacecraft); Sky; Galaxy; Sunyaev–Zel'dovich effect; Astronomy; Cosmic microwave background; Computer science","score_opus":0.009262560563020081,"score_gpt":0.1888524954811819,"score_spread":0.17958993491816183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045643973","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927286,0.00005253489,0.001838521,0.000042006952,0.0000060085504,0.00002000483,0.0033687274,0.00012381337,0.001819734],"genre_scores_gemma":[0.9884431,0.00006104726,0.004532334,0.00002708176,0.000021860478,0.00003253582,0.0061959825,0.000039095816,0.00064694346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995788,0.00007121084,0.00002179335,0.00016614844,0.000098153396,0.0000639054],"domain_scores_gemma":[0.9978992,0.00037874168,0.00052158866,0.00049499393,0.00021045569,0.00049500907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076296576,0.00024356633,0.0002359733,0.001660853,0.00036804384,0.0007419272,0.00042795544,0.0002341798,0.0017978221],"category_scores_gemma":[0.0031520172,0.0002491534,0.00018921556,0.0016755995,0.0002644624,0.0010635898,0.001176501,0.00024440847,0.00048379923],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003901946,0.00010471802,0.9486181,0.00006519526,0.00020706821,0.000101947764,0.0009171337,0.005489837,0.00602444,0.0028333927,0.003746002,0.03150193],"study_design_scores_gemma":[0.000015253481,0.00004217771,0.9857209,0.000008383029,0.000041741583,0.000071608214,0.00020489749,0.00807532,0.0019088485,0.00086139404,0.0030239348,0.000025447223],"about_ca_topic_score_codex":0.008448119,"about_ca_topic_score_gemma":0.009740045,"teacher_disagreement_score":0.008448119,"about_ca_system_score_codex":0.00040314166,"about_ca_system_score_gemma":0.00030091114,"threshold_uncertainty_score":0.0167979},"labels":[],"label_agreement":null},{"id":"W2045651420","doi":"10.1088/0004-637x/749/1/6","title":"DETAILED COMPOSITIONAL ANALYSIS OF THE HEAVILY POLLUTED DBZ WHITE DWARF SDSS J073842.56+183509.06: A WINDOW ON PLANET FORMATION?","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":131,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planet; White dwarf; Atmosphere (unit); Debris; Parent body; Line (geometry); Window (computing)","score_opus":0.010183975688001693,"score_gpt":0.22345499969651236,"score_spread":0.21327102400851067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045651420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983016,0.00006220701,0.0003771519,0.00002554271,0.0000023552434,0.0000033479223,0.00064272113,0.000043623586,0.0005413894],"genre_scores_gemma":[0.99646807,0.000072990515,0.0008908464,0.00002202422,0.0000070184487,0.0000037872671,0.0020934446,0.000027772432,0.00041401194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999449,0.000004615261,0.0000024244434,0.00001947834,0.000012613601,0.000015949041],"domain_scores_gemma":[0.9999411,0.0000035705523,0.000014295563,0.000012086132,0.000010514724,0.00001838281],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000091064445,0.00032036516,0.00028054055,0.00048339315,0.0003252854,0.0004410765,0.0002834128,0.00025641854,0.00080805895],"category_scores_gemma":[0.00012638874,0.0001294105,0.00034402224,0.00036433592,0.00016545245,0.00028508843,0.00030237954,0.0001630845,0.0003523879],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024249991,0.000113214424,0.79477006,0.000062827596,0.0001678118,0.0005059659,0.00045261593,0.0109006595,0.17796986,0.001002482,0.0009025466,0.012909472],"study_design_scores_gemma":[0.000017844994,0.00008188243,0.95963365,0.000004363563,0.00004593998,0.00017215859,0.0002619483,0.026382022,0.0076930746,0.0005151265,0.0051768194,0.000015198586],"about_ca_topic_score_codex":0.0144032985,"about_ca_topic_score_gemma":0.02040191,"teacher_disagreement_score":0.0144032985,"about_ca_system_score_codex":0.00052165147,"about_ca_system_score_gemma":0.00019923193,"threshold_uncertainty_score":0.0286389},"labels":[],"label_agreement":null},{"id":"W2045752989","doi":"10.1086/498263","title":"The Role of the 96 keV Level in the<sup>19</sup>O(β<sup>-</sup>)<sup>19</sup>F Process at Stellar Temperatures","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"","keywords":"Physics; Excited state; Atomic physics; Nucleosynthesis; Nuclear reaction; Excitation; Ground state; r-process; s-process; Nuclear physics; Isobaric process; Radioactive decay; Beta decay","score_opus":0.014609388272319895,"score_gpt":0.27268472537375144,"score_spread":0.25807533710143155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045752989","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940165,0.00017543732,0.002908853,0.00003900357,0.0000042320917,0.0000042400093,0.000057191624,0.000024831526,0.0027696448],"genre_scores_gemma":[0.99875355,0.000076949334,0.0005315023,0.0000038982766,0.0000019002542,0.0000026204982,0.00003892858,0.000017359389,0.0005732548],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999249,0.000017796021,0.0000032167363,0.000019641822,0.000013715759,0.0000206786],"domain_scores_gemma":[0.99925214,0.0003969418,0.00019811737,0.00004594286,0.00006244393,0.000044407043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045945615,0.0003951996,0.00017241004,0.0003542384,0.0004197215,0.0007175089,0.00039476334,0.00027959907,0.0023264727],"category_scores_gemma":[0.0012141169,0.00017613043,0.00029952067,0.00017091645,0.0005354612,0.0005946788,0.00031619807,0.00038426297,0.0004527349],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0029452504,0.00017988749,0.121873185,0.00032736006,0.00008177932,0.0020086796,0.0012645922,0.053573374,0.7302177,0.06511149,0.00025162933,0.022165142],"study_design_scores_gemma":[0.000157567,0.0011095711,0.100154586,0.00014587276,0.00017810344,0.004035662,0.0008129576,0.20079045,0.66139054,0.027397826,0.0037401896,0.00008666694],"about_ca_topic_score_codex":0.000575161,"about_ca_topic_score_gemma":0.00041073575,"teacher_disagreement_score":0.0023264727,"about_ca_system_score_codex":0.00040437814,"about_ca_system_score_gemma":0.0001278022,"threshold_uncertainty_score":0.0077827573},"labels":[],"label_agreement":null},{"id":"W2045767679","doi":"10.1088/0004-637x/797/2/138","title":"LENS MODELS OF<i>HERSCHEL</i>-SELECTED GALAXIES FROM HIGH-RESOLUTION NEAR-IR OBSERVATIONS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Smithsonian Astrophysical Observatory; Centre National de la Recherche Scientifique; Danmarks Grundforskningsfond; Science and Technology Facilities Council; National Research Foundation; James S. McDonnell Foundation; Kenneth T. and Eileen L. Norris Foundation; UK Space Agency; Key Programme; Centre National d’Etudes Spatiales; Aspen Center for Physics; University of Chicago; Gordon and Betty Moore Foundation; Space Telescope Science Institute; W. M. Keck Foundation; Imperial College London; National Science Foundation; Academia Sinica; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Magnification; Adaptive optics; Optics","score_opus":0.015319136232341289,"score_gpt":0.20037482508324558,"score_spread":0.1850556888509043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045767679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9747883,0.0004468054,0.016801873,0.0001859129,0.0000052817445,0.000025870384,0.001686982,0.00026452646,0.005794523],"genre_scores_gemma":[0.9928034,0.00021058472,0.0040654377,0.0000284654,0.000009725237,0.000012858264,0.0013974084,0.00002895395,0.001443221],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998969,0.000019578883,0.0000075369526,0.000035057386,0.0000207031,0.000020161584],"domain_scores_gemma":[0.999509,0.0001469833,0.00018759638,0.00004803042,0.000043900844,0.00006462417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003163075,0.0004655773,0.00025511612,0.00074213505,0.00022953887,0.0008524371,0.00087606185,0.0004042627,0.002406508],"category_scores_gemma":[0.0009304349,0.00032839447,0.0004716608,0.00053171034,0.0002536415,0.0010060454,0.00037672618,0.00021111904,0.0005511703],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001363546,0.0000344156,0.06555472,0.000062320076,0.00016470045,0.00020373803,0.00013734582,0.91307193,0.0039516124,0.0052991095,0.0008291415,0.0105547],"study_design_scores_gemma":[0.000027061085,0.00003224417,0.028407479,0.000010685545,0.000036098536,0.00007706855,0.000051241965,0.96648484,0.00084726466,0.003182542,0.0008200153,0.000023405575],"about_ca_topic_score_codex":0.038453348,"about_ca_topic_score_gemma":0.03958017,"teacher_disagreement_score":0.038453348,"about_ca_system_score_codex":0.0022921055,"about_ca_system_score_gemma":0.0003713097,"threshold_uncertainty_score":0.07645905},"labels":[],"label_agreement":null},{"id":"W2045775572","doi":"10.1088/0004-637x/718/2/1416","title":"MODELING THE NEAR-ULTRAVIOLET BAND OF GK STARS. I. LOCAL THERMODYNAMIC EQUILIBRIUM MODELS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Metallicity; Stars; Spectral line; Luminosity; Effective temperature; Stellar atmosphere; Line (geometry); Standard solar model; Astronomy; Atmospheric models; Galaxy","score_opus":0.010824130784555372,"score_gpt":0.21912061411877323,"score_spread":0.20829648333421785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045775572","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8880011,0.00027218965,0.08203828,0.00039580255,0.000033296765,0.000071725386,0.0024049375,0.0006512526,0.026131343],"genre_scores_gemma":[0.98347455,0.00013978883,0.010134432,0.000096483855,0.00001620426,0.000089923415,0.0008724458,0.00016337483,0.0050127446],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988866,0.000027549298,0.0000057537573,0.000032591783,0.000018417328,0.000026979214],"domain_scores_gemma":[0.999803,0.000056637797,0.000035582427,0.000032070653,0.00003840559,0.000034241257],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022427582,0.00045412628,0.00044895711,0.0004353468,0.00055437844,0.0010218814,0.0015835207,0.00071522256,0.0029545017],"category_scores_gemma":[0.001174543,0.000308004,0.0006653639,0.0005382223,0.0005720876,0.0014169567,0.00072812295,0.0006350181,0.00093065517],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049756516,0.00004103674,0.013601522,0.000030585827,0.000042553118,0.000064001084,0.00014339111,0.96475416,0.001763291,0.016318044,0.00058038405,0.0026113088],"study_design_scores_gemma":[0.000020928086,0.000017283011,0.0021227351,0.0000055662767,0.00001083544,0.000031789354,0.00005232219,0.98924875,0.00034526948,0.007073014,0.0010598558,0.00001166867],"about_ca_topic_score_codex":0.02482678,"about_ca_topic_score_gemma":0.015246594,"teacher_disagreement_score":0.02482678,"about_ca_system_score_codex":0.0012357562,"about_ca_system_score_gemma":0.0006069955,"threshold_uncertainty_score":0.049364507},"labels":[],"label_agreement":null},{"id":"W2045805552","doi":"10.1086/378345","title":"Indications for Grain Growth and Mass Decrease in Cold Dust Disks around Classical T Tauri Stars in the MBM 12 Young Association","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"T Tauri star; Stars; Grain growth; Grain size; Accretion (finance); Cosmic dust; Accretion disc","score_opus":0.011585077470279159,"score_gpt":0.24257143402846906,"score_spread":0.23098635655818991,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045805552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99920076,0.00009941326,0.000043868433,0.000024086843,0.000006375339,0.0000026509313,0.00014665196,0.000008814757,0.00046743706],"genre_scores_gemma":[0.998946,0.000046815894,0.0000659982,0.000021619875,0.000025577901,0.0000035884636,0.00019663911,0.000005967649,0.000687785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999126,0.000004828779,0.000009510783,0.000023490951,0.000021069649,0.00002839398],"domain_scores_gemma":[0.9984377,0.00022432218,0.0004798967,0.000075250966,0.0003451023,0.00043773255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016050159,0.0001751936,0.00031462387,0.0012214972,0.00058759336,0.0007537772,0.00034971803,0.0006581208,0.0040068934],"category_scores_gemma":[0.0009926797,0.00020153383,0.00021524885,0.0005287311,0.00038711893,0.00041301048,0.0003870765,0.00037207984,0.0008957398],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009656977,0.00009376368,0.940762,0.00005110011,0.00003197083,0.0006110874,0.0005094052,0.000057642905,0.051790718,0.000055772318,0.0003654035,0.004705532],"study_design_scores_gemma":[0.0000057418247,0.00003881197,0.99879754,0.0000012028449,0.0000062970503,0.0001548414,0.00012092988,0.000028952594,0.0007340825,0.000015168881,0.00009500209,0.0000014567659],"about_ca_topic_score_codex":0.0034708078,"about_ca_topic_score_gemma":0.0046364954,"teacher_disagreement_score":0.0040068934,"about_ca_system_score_codex":0.00018587487,"about_ca_system_score_gemma":0.00011472839,"threshold_uncertainty_score":0.013404369},"labels":[],"label_agreement":null},{"id":"W2045815794","doi":"10.1088/0004-637x/719/1/803","title":"THE DISCOVERY OF THE MOST METAL-RICH WHITE DWARF: COMPOSITION OF A TIDALLY DISRUPTED EXTRASOLAR DWARF PLANET","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Exoplanet; Physics; Astrophysics; Atmosphere (unit); Stars; Planet; Dwarf planet; Photometry (optics); Astronomy; Astrobiology","score_opus":0.004796533106190184,"score_gpt":0.2030761974961008,"score_spread":0.19827966438991063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045815794","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99901295,0.00010220631,0.00029671215,0.000015955799,8.077169e-7,0.0000011324388,0.000107361026,0.000012883992,0.00044993963],"genre_scores_gemma":[0.9992768,0.00007524471,0.0003007367,0.0000063205207,0.0000023516473,5.8372115e-7,0.00018026285,0.0000026007533,0.00015511588],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999721,0.0000025415038,0.000001844932,0.000012309129,0.000007805235,0.000003494031],"domain_scores_gemma":[0.9999267,0.0000049093733,0.00003491786,0.000009627067,0.0000069376883,0.000016884738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000666523,0.00015947263,0.00013596436,0.00045645752,0.00030368744,0.0003864165,0.00014662214,0.0002151559,0.0004945431],"category_scores_gemma":[0.00014862815,0.00008183492,0.0000881056,0.000446047,0.00021436652,0.00028625657,0.00026782017,0.000104970924,0.00017818871],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010358229,0.00003323279,0.76328754,0.00004468934,0.000039749033,0.00028620055,0.00021200265,0.0003965784,0.22630244,0.00033470496,0.00011465548,0.008844626],"study_design_scores_gemma":[0.000002316198,0.000051997522,0.9868527,0.0000025314262,0.000018394674,0.0004692789,0.000106461775,0.0008683023,0.010524564,0.00016583806,0.0009352898,0.0000023907387],"about_ca_topic_score_codex":0.0012472336,"about_ca_topic_score_gemma":0.0022979982,"teacher_disagreement_score":0.0012472336,"about_ca_system_score_codex":0.00017097709,"about_ca_system_score_gemma":0.00008301872,"threshold_uncertainty_score":0.0024799109},"labels":[],"label_agreement":null},{"id":"W2045903795","doi":"10.1088/0004-637x/735/2/101","title":"OBSERVATIONAL EVIDENCE AGAINST LONG-LIVED SPIRAL ARMS IN GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Spiral galaxy; Stars; Tracing; Galaxy; Density wave theory; Spiral (railway); Star formation; Barred spiral galaxy","score_opus":0.05585893869294252,"score_gpt":0.25006142116123825,"score_spread":0.19420248246829575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045903795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976549,0.00020340124,0.0004746594,0.00005209597,0.0000028686907,0.000001972209,0.00011068293,0.000032501706,0.001466842],"genre_scores_gemma":[0.99964464,0.000032363456,0.00013015259,0.000008464278,0.0000047960607,9.348364e-7,0.00011416286,0.0000031638258,0.000061345796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995733,0.00007086088,0.000033593446,0.00011012767,0.0001309291,0.000081133614],"domain_scores_gemma":[0.9892447,0.0028939836,0.0043070335,0.0011907461,0.001221049,0.001142507],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006383866,0.00018402745,0.00016959257,0.0013149362,0.00036817155,0.0010826343,0.0005089265,0.00044716836,0.0020221043],"category_scores_gemma":[0.0066120066,0.00019526298,0.0002195109,0.0009595471,0.0012211981,0.00056523527,0.0008309021,0.00033396037,0.00035067572],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000072869894,0.000009809893,0.9940162,0.000010989304,0.000042477164,0.00005113619,0.00017561269,0.00035136592,0.001771226,0.00048129214,0.00007029215,0.0029467917],"study_design_scores_gemma":[0.0000069137104,0.00003717691,0.9974491,0.000010526056,0.00002112009,0.00014396437,0.0001588965,0.000976253,0.0003960452,0.00042700596,0.00036808598,0.0000048106294],"about_ca_topic_score_codex":0.0041911383,"about_ca_topic_score_gemma":0.0062238015,"teacher_disagreement_score":0.0041911383,"about_ca_system_score_codex":0.00041811896,"about_ca_system_score_gemma":0.00017248964,"threshold_uncertainty_score":0.008333445},"labels":[],"label_agreement":null},{"id":"W2045997953","doi":"10.1088/0004-637x/778/2/87","title":"INTERACTIONS OF COSMIC RAYS IN THE ATMOSPHERE: GROWTH CURVES REVISITED","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radiation Therapy and Dosimetry","field":"Medicine","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cosmic ray; Extrapolation; Physics; Atmosphere (unit); COSMIC cancer database; Nuclear physics; Computational physics; Astrophysics; Statistics; Meteorology","score_opus":0.010904929003911492,"score_gpt":0.26541767318356396,"score_spread":0.2545127441796525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2045997953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9245433,0.00477564,0.034769423,0.0010161662,0.000036903246,0.00006306652,0.0027932983,0.001004341,0.030997816],"genre_scores_gemma":[0.98774195,0.0008195444,0.007211496,0.000054340075,0.000013292816,0.000027267675,0.0010996397,0.00026024866,0.0027722768],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99945325,0.00010516436,0.000019072277,0.00010491583,0.00023482792,0.000082835206],"domain_scores_gemma":[0.99640214,0.0013928761,0.00067254883,0.0004036421,0.0009496792,0.00017912636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010812382,0.00067591213,0.00033600716,0.0016638379,0.00036868048,0.00065897434,0.00076856575,0.00054716365,0.0018524273],"category_scores_gemma":[0.0048056687,0.00025674855,0.0007214397,0.0017375833,0.00064512057,0.0010180203,0.0009003313,0.0009642692,0.0007769172],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000880469,0.00013304564,0.54030335,0.0005114047,0.00029485015,0.0012624133,0.003432137,0.06529126,0.14992283,0.036044206,0.005944475,0.19597957],"study_design_scores_gemma":[0.000029891477,0.00041605675,0.6437998,0.00012676169,0.00011250993,0.003078806,0.0010032818,0.19541691,0.09129273,0.02074424,0.04382711,0.00015190948],"about_ca_topic_score_codex":0.0098674465,"about_ca_topic_score_gemma":0.0043846504,"teacher_disagreement_score":0.0098674465,"about_ca_system_score_codex":0.0011278597,"about_ca_system_score_gemma":0.00043223493,"threshold_uncertainty_score":0.01962006},"labels":[],"label_agreement":null},{"id":"W2046014239","doi":"10.1088/0004-637x/696/1/924","title":"X-RAY INSIGHTS INTO THE PHYSICS OF MINI-BAL QUASAR OUTFLOWS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"QSOS; Astrophysics; Physics; Quasar; Population; Astronomy; Sky; Brightness; X-ray; Absorption (acoustics); Galaxy; Medicine; Optics","score_opus":0.007849463403354068,"score_gpt":0.21701103548724662,"score_spread":0.20916157208389255,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046014239","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99760133,0.0006872563,0.0007960745,0.000039669794,0.000002217312,0.0000044908124,0.000063242886,0.000020465726,0.00078521826],"genre_scores_gemma":[0.9991523,0.00022244497,0.00029007395,0.0000267559,0.000012341523,0.0000019855847,0.00008154818,0.0000032459861,0.00020928401],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999331,0.0000123568225,0.0000066631965,0.000014221992,0.000011190192,0.000022452308],"domain_scores_gemma":[0.99919957,0.00022725922,0.00033888916,0.000057324385,0.000057165955,0.00011983373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031854602,0.0002693841,0.00018190693,0.00090920634,0.00016458562,0.00046231458,0.00023671381,0.00021889039,0.0014243299],"category_scores_gemma":[0.00072035077,0.00014820628,0.00015760043,0.0005011255,0.00030844833,0.0008311088,0.00052328565,0.00024013405,0.00020740814],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017176173,0.00006712534,0.95387626,0.000068447436,0.000037852573,0.00061439653,0.0004181745,0.0013103964,0.032011434,0.0015012582,0.000115254676,0.009807609],"study_design_scores_gemma":[0.0000038132614,0.00008323954,0.9941619,0.000008339635,0.00001279063,0.0007166044,0.0002248619,0.002031367,0.0011196459,0.0009158385,0.0007171148,0.000004456182],"about_ca_topic_score_codex":0.0003903249,"about_ca_topic_score_gemma":0.00062958786,"teacher_disagreement_score":0.0014243299,"about_ca_system_score_codex":0.00014376084,"about_ca_system_score_gemma":0.00006680979,"threshold_uncertainty_score":0.0047649145},"labels":[],"label_agreement":null},{"id":"W2046229226","doi":"10.1086/425866","title":"Surface Brightness and Stellar Populations at the Outer Edge of the Large Magellanic Cloud: No Stellar Halo Yet","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Surface brightness; Astronomy; Large Magellanic Cloud; Halo; Stellar population; Population; Galaxy; Star formation; Stellar density; RADIUS; Stars","score_opus":0.013407773201994612,"score_gpt":0.23041158841267875,"score_spread":0.21700381521068415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046229226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99674016,0.00016558009,0.0003541167,0.000027933995,0.0000020185246,0.0000029084554,0.0010368216,0.000037970054,0.0016325113],"genre_scores_gemma":[0.9977149,0.000037270143,0.00049708027,0.0000103755265,0.0000068216345,0.0000014501123,0.0013103016,0.000010757021,0.0004111827],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998926,0.0000047758726,0.0000036548774,0.000031802116,0.000025483992,0.000041668918],"domain_scores_gemma":[0.9996018,0.000044376473,0.000083540945,0.00006481688,0.00005336707,0.00015212334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012421612,0.00021928643,0.000298565,0.0012751726,0.00026688445,0.00044991594,0.00027134782,0.0002182402,0.002346184],"category_scores_gemma":[0.0003772162,0.00011187774,0.00011359018,0.0007674609,0.00022705548,0.000296013,0.00042745497,0.00019215529,0.00058318203],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036147665,0.000056288358,0.90930766,0.00004985969,0.00003536667,0.0003634818,0.00025784862,0.00070640986,0.06832607,0.00025013863,0.00040690158,0.019878417],"study_design_scores_gemma":[0.000003193578,0.000027364265,0.99712294,0.000002744836,0.0000069714984,0.00024429546,0.0000419386,0.00041706208,0.0014387841,0.000045113768,0.0006467175,0.0000027803023],"about_ca_topic_score_codex":0.0093517015,"about_ca_topic_score_gemma":0.01331489,"teacher_disagreement_score":0.0093517015,"about_ca_system_score_codex":0.00034410425,"about_ca_system_score_gemma":0.00011979375,"threshold_uncertainty_score":0.018594563},"labels":[],"label_agreement":null},{"id":"W2046258798","doi":"10.1088/0004-637x/753/1/70","title":"<i>HERSCHEL</i>-SPIRE IMAGING SPECTROSCOPY OF MOLECULAR GAS IN M82","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Radiative transfer; Spectroscopy; Line (geometry); Spectral line; Galaxy; Emission spectrum; Absorption (acoustics); Absorption spectroscopy","score_opus":0.00480415278555347,"score_gpt":0.21642216666782108,"score_spread":0.2116180138822676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046258798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5937981,0.015432954,0.018151041,0.067589946,0.0040960046,0.0002893583,0.05188455,0.013182408,0.23557565],"genre_scores_gemma":[0.9193123,0.0017344012,0.010973442,0.0072774044,0.0020015594,0.0001216602,0.016482117,0.0010642287,0.041032918],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99982494,0.00001571749,0.000006882184,0.000045193112,0.000054590713,0.000052688065],"domain_scores_gemma":[0.99961674,0.00007063051,0.000053753058,0.000044225926,0.000081605154,0.00013300456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000986792,0.00042720302,0.00034840195,0.0019423659,0.0007984514,0.0012204534,0.0007284848,0.0013666345,0.015016695],"category_scores_gemma":[0.0006896845,0.0003024303,0.00040819935,0.00081399275,0.00032561706,0.0008231763,0.0011594307,0.000949284,0.0027180328],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093260925,0.00026898773,0.061639726,0.00074099744,0.00034820623,0.001783849,0.0006661594,0.0032447819,0.46754128,0.003998478,0.38219708,0.0766378],"study_design_scores_gemma":[0.0002592048,0.00026088074,0.75670105,0.0003158205,0.00042431793,0.0016785135,0.0009231973,0.012163014,0.07201242,0.0062767123,0.14872673,0.00025815805],"about_ca_topic_score_codex":0.004296572,"about_ca_topic_score_gemma":0.0150713045,"teacher_disagreement_score":0.015016695,"about_ca_system_score_codex":0.00062284403,"about_ca_system_score_gemma":0.00049016986,"threshold_uncertainty_score":0.050235868},"labels":[],"label_agreement":null},{"id":"W2046265078","doi":"10.1088/0004-637x/744/2/125","title":"DRIFT COEFFICIENTS OF CHARGED PARTICLES IN TURBULENT MAGNETIC FIELDS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Turbulence; Magnetohydrodynamic turbulence; K-epsilon turbulence model; K-omega turbulence model; Computational physics; Scattering; Classical mechanics; Diffusion; Magnetohydrodynamics; Tensor (intrinsic definition); Range (aeronautics); Astron; Mechanics; Plasma; Statistical physics; Astrophysics; Optics; Geometry; Quantum mechanics","score_opus":0.011736576810865975,"score_gpt":0.21292093761872874,"score_spread":0.20118436080786276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046265078","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9470897,0.00053167937,0.042463016,0.00026570546,0.00015107726,0.00006820368,0.0003243322,0.00015463914,0.008951817],"genre_scores_gemma":[0.99300164,0.00023988883,0.005085806,0.00003084527,0.000013919011,0.000026122996,0.00017221361,0.000045206885,0.0013842392],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986684,0.00003006158,0.000011094203,0.000014696365,0.000039771494,0.000037508446],"domain_scores_gemma":[0.9992772,0.00030192334,0.000101889265,0.000035377798,0.00018849678,0.00009524298],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065999915,0.00053601933,0.00041954292,0.0008928967,0.0007721937,0.0011556481,0.00057314767,0.0006831644,0.0008703637],"category_scores_gemma":[0.0026575094,0.0003036457,0.00034142245,0.00086090434,0.00087957823,0.0008676386,0.00063511863,0.000505753,0.0001638489],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018173123,0.000058526173,0.004371425,0.00010251015,0.000041350162,0.00037584908,0.00021958842,0.9487434,0.013622164,0.027341252,0.0005419752,0.0044001765],"study_design_scores_gemma":[0.000036613823,0.0000212077,0.00076098973,0.000011485801,0.0000056311387,0.000035584155,0.000036042602,0.9928913,0.0036969625,0.0022149729,0.00026810105,0.000021140397],"about_ca_topic_score_codex":0.0096608875,"about_ca_topic_score_gemma":0.0045071323,"teacher_disagreement_score":0.0096608875,"about_ca_system_score_codex":0.0012567162,"about_ca_system_score_gemma":0.0012948822,"threshold_uncertainty_score":0.019209325},"labels":[],"label_agreement":null},{"id":"W2046325489","doi":"10.1086/589140","title":"Pair Analysis of Field Galaxies from the Red‐Sequence Cluster Survey","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Redshift; Galaxy; Luminosity; Absolute magnitude; Redshift survey; Galaxy cluster; Cosmology; Cluster (spacecraft); Cluster sampling; Magnitude (astronomy); Astronomy; Population","score_opus":0.020264358781548038,"score_gpt":0.2313617994593801,"score_spread":0.21109744067783207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046325489","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99890256,0.000053341846,0.00025286226,0.000006973286,9.540914e-7,0.0000038202074,0.0005271413,0.000013934772,0.00023843792],"genre_scores_gemma":[0.9970944,0.000024640161,0.0004312007,0.00000434748,0.0000027181406,0.000006279817,0.0020231635,0.000006420639,0.000406757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996172,0.00007072761,0.000011413932,0.00014116448,0.000063016145,0.00009634222],"domain_scores_gemma":[0.9987734,0.00028455062,0.00032413498,0.00018278329,0.00017325557,0.0002619199],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005293304,0.00024055685,0.00041810478,0.0021119919,0.00039804,0.0004155645,0.0004287245,0.00026409328,0.0015872824],"category_scores_gemma":[0.0012813201,0.00017995438,0.00044673381,0.0011944625,0.0001974953,0.00025471457,0.00054148026,0.00018382208,0.0003744972],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020533173,0.000028596347,0.9895363,0.000015692116,0.00010117432,0.00013686587,0.00012527723,0.0016989058,0.002410416,0.0002274708,0.00047615854,0.005037793],"study_design_scores_gemma":[0.000008505054,0.00004329929,0.9907575,0.00000172759,0.000037158326,0.00014207733,0.00007116774,0.0077671376,0.0006422236,0.000067297166,0.00045551502,0.000006319135],"about_ca_topic_score_codex":0.015449309,"about_ca_topic_score_gemma":0.017694496,"teacher_disagreement_score":0.015449309,"about_ca_system_score_codex":0.0005005987,"about_ca_system_score_gemma":0.0002730945,"threshold_uncertainty_score":0.030718803},"labels":[],"label_agreement":null},{"id":"W2046372280","doi":"10.1086/510151","title":"Deviations from He<scp>i</scp>Case B Recombination Theory and Extinction Corrections in the Orion Nebula","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Extinction (optical mineralogy); Radiative transfer; Physics; Photoionization; Orion Nebula; Astrophysics; Nebula; Wavelength; Molar absorptivity; Radiative equilibrium; Recombination; Lambda; Series (stratigraphy); Optics; Chemistry; Stars; Ion; Biology; Ionization","score_opus":0.009759469764131052,"score_gpt":0.24703324555779257,"score_spread":0.23727377579366152,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046372280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9442244,0.000684525,0.046215177,0.00051029434,0.000044578435,0.00003056144,0.00008317506,0.0003845123,0.007822815],"genre_scores_gemma":[0.9956404,0.000092592054,0.0036277212,0.000040867577,0.00001236421,0.000010557502,0.000056381927,0.00004483018,0.00047432474],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9994104,0.00010697848,0.00003421309,0.00019272367,0.00019005034,0.000065726825],"domain_scores_gemma":[0.9983346,0.0005408143,0.00046700964,0.00034956264,0.00023436653,0.00007370381],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019913255,0.00043469804,0.00033466125,0.0007322567,0.00045985373,0.0008674712,0.0014016379,0.00046322774,0.0007274876],"category_scores_gemma":[0.0059032734,0.00018113549,0.00040407854,0.0003549811,0.00079591037,0.0010548523,0.0008754628,0.00054825656,0.00017844426],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071771233,0.00031270977,0.26899874,0.00022762339,0.0002859,0.0016429407,0.00081864826,0.2861113,0.07381021,0.26564154,0.0020088288,0.099423915],"study_design_scores_gemma":[0.00007183486,0.00019866123,0.08361508,0.000042990392,0.000052418454,0.0007651148,0.00027141886,0.79740566,0.017827345,0.09716774,0.0025293413,0.000052475378],"about_ca_topic_score_codex":0.0063266554,"about_ca_topic_score_gemma":0.0020409836,"teacher_disagreement_score":0.0063266554,"about_ca_system_score_codex":0.00090420333,"about_ca_system_score_gemma":0.0005242267,"threshold_uncertainty_score":0.01257962},"labels":[],"label_agreement":null},{"id":"W2046386183","doi":"10.1086/426470","title":"Implications of<i>WMAP</i>Observations on Li Abundance and Stellar Evolution Models","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":267,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Stellar evolution; Abundance (ecology); Stellar atmosphere; Stars; Galaxy formation and evolution; Chemical evolution; Stellar physics; Stellar collision","score_opus":0.016753138836628136,"score_gpt":0.25043372132249025,"score_spread":0.23368058248586213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046386183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.61947805,0.009780783,0.02921731,0.18769298,0.00378533,0.000058509646,0.011505173,0.0012632401,0.13721864],"genre_scores_gemma":[0.980445,0.0017046744,0.0024850385,0.0075767064,0.0014077205,0.00003307583,0.0017824552,0.00014470563,0.004420649],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996216,0.00011892747,0.000022245109,0.00011945512,0.00006300578,0.000054616212],"domain_scores_gemma":[0.9962482,0.001956825,0.0005237336,0.0004325969,0.00046522034,0.00037343628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002920638,0.0009291923,0.0008655425,0.001044172,0.001317614,0.0038791941,0.002586077,0.0023342185,0.01911648],"category_scores_gemma":[0.008855341,0.00048328968,0.0010448861,0.0017229231,0.001465657,0.0040082084,0.0017785752,0.0020361373,0.0018461831],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021337853,0.00029296614,0.10304944,0.0012603881,0.0013291254,0.0023395875,0.0018919186,0.09226797,0.017782668,0.5844172,0.10960651,0.08362842],"study_design_scores_gemma":[0.00022322727,0.000071309754,0.040220205,0.00024742112,0.00023501395,0.00030926077,0.0013600448,0.063651964,0.0044089416,0.8674059,0.021693496,0.000173113],"about_ca_topic_score_codex":0.013405374,"about_ca_topic_score_gemma":0.005636991,"teacher_disagreement_score":0.01911648,"about_ca_system_score_codex":0.0018969879,"about_ca_system_score_gemma":0.0007807784,"threshold_uncertainty_score":0.063951015},"labels":[],"label_agreement":null},{"id":"W2046394178","doi":"10.1088/0004-637x/763/2/96","title":"STACKING STAR CLUSTERS IN M51: SEARCHING FOR FAINT X-RAY BINARIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Astrophysics; Star (game theory); Stacking; Astronomy; Physics; Star cluster; Galaxy","score_opus":0.01764727966954435,"score_gpt":0.24973432117458016,"score_spread":0.2320870415050358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046394178","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99948287,0.000065526176,0.00018277677,0.000007638553,6.9118335e-7,0.0000028490945,0.000027813428,0.000008379467,0.0002215084],"genre_scores_gemma":[0.9990113,0.000039681945,0.00060346926,0.0000060881744,0.0000022360732,0.0000019901765,0.0001421534,0.0000021179762,0.00019096221],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981993,0.00002941335,0.000016961998,0.000054120585,0.000036186353,0.00004336924],"domain_scores_gemma":[0.9993875,0.00011332234,0.00021769915,0.00006741305,0.00006521558,0.00014891793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043876815,0.0003216324,0.00028950264,0.0017720762,0.0005996727,0.0006082707,0.00030860628,0.00029344053,0.0017668811],"category_scores_gemma":[0.001096531,0.00019081026,0.00019630014,0.0011730884,0.00029585892,0.00040872733,0.00087397906,0.0001343922,0.000524192],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014438161,0.000030946496,0.97220343,0.000017355653,0.00003236596,0.00023543603,0.00046238018,0.00044437184,0.012705728,0.00028429818,0.00012690783,0.013312251],"study_design_scores_gemma":[0.0000037808586,0.000076255536,0.9967933,0.00000428927,0.00001755288,0.00023460758,0.000191747,0.0011612527,0.0010994882,0.00015957413,0.00025343383,0.000004624583],"about_ca_topic_score_codex":0.0042987387,"about_ca_topic_score_gemma":0.0060933963,"teacher_disagreement_score":0.0042987387,"about_ca_system_score_codex":0.00027051193,"about_ca_system_score_gemma":0.00021014661,"threshold_uncertainty_score":0.008547425},"labels":[],"label_agreement":null},{"id":"W2046409070","doi":"10.1088/0004-637x/721/1/493","title":"THE EVOLUTION OF CLOUD CORES AND THE FORMATION OF STARS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Stars; Physics; Instability; Dissipation; Astrophysics; Amplitude; Star formation; Mechanics","score_opus":0.005113733361714136,"score_gpt":0.2170195748170832,"score_spread":0.21190584145536906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046409070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99835384,0.0003288482,0.00013240929,0.00004642762,0.0000019462718,0.0000023485634,0.00004103116,0.000002281191,0.0010910487],"genre_scores_gemma":[0.9996637,0.00006954639,0.00007002703,0.000008125931,0.0000020460323,6.177365e-7,0.000038877537,0.0000010113748,0.00014608688],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999167,0.000015127437,0.000005496578,0.000018063916,0.000014166745,0.000030468054],"domain_scores_gemma":[0.99948126,0.000070437454,0.00023928244,0.00002009421,0.000054194687,0.00013473212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026840094,0.00010697577,0.0001163428,0.0005340297,0.00043264264,0.0008118168,0.00017904401,0.00032038442,0.0006398948],"category_scores_gemma":[0.0012041981,0.00011322023,0.00010320688,0.00032512075,0.00036630745,0.00044483787,0.00044821325,0.00019515949,0.0001385871],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021900496,0.00005952482,0.9484413,0.000031232157,0.000045802815,0.00038220847,0.0003520101,0.00447991,0.028188515,0.0061402246,0.00022981748,0.011430439],"study_design_scores_gemma":[0.000010628207,0.000041955034,0.9897558,0.0000093160215,0.000010892706,0.00018284358,0.0001804585,0.0052660056,0.0018809803,0.0016679071,0.0009871755,0.000005976913],"about_ca_topic_score_codex":0.006807357,"about_ca_topic_score_gemma":0.0073988554,"teacher_disagreement_score":0.006807357,"about_ca_system_score_codex":0.00094303145,"about_ca_system_score_gemma":0.00030512718,"threshold_uncertainty_score":0.01353544},"labels":[],"label_agreement":null},{"id":"W2046417299","doi":"10.1086/375052","title":"The Nearby Neutron Star RX J0720.4−3125 from Radio to X‐Rays","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Pulsar; Neutron star; Black-body radiation; RADIUS; Luminosity; Flux (metallurgy); Limit (mathematics)","score_opus":0.01039410831910507,"score_gpt":0.2917131834210553,"score_spread":0.2813190751019502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046417299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959889,0.00034015774,0.00017193802,0.000023391276,0.0000071050868,0.0000062850345,0.00022838863,0.000025164292,0.0032085942],"genre_scores_gemma":[0.9972928,0.0001921505,0.00041840287,0.000044469,0.000012940181,0.0000038147896,0.0011636615,0.0000067733095,0.0008650225],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993074,0.000004773273,0.000005027326,0.000022482167,0.000020017711,0.000016957521],"domain_scores_gemma":[0.9998672,0.000005743212,0.000044459895,0.000014208366,0.000012449522,0.000056007866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009541709,0.00027951325,0.00025217087,0.0006263094,0.0005116545,0.00049193355,0.00030070377,0.00021400586,0.0018170496],"category_scores_gemma":[0.00020780363,0.000112689326,0.00020224992,0.00069571857,0.00017933482,0.00023100396,0.00067295926,0.00017741343,0.0005547337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013734621,0.00023819895,0.6751279,0.00035759294,0.00015128369,0.0031008055,0.0014235812,0.0046385196,0.25130686,0.0025633883,0.002155253,0.057563197],"study_design_scores_gemma":[0.000025416623,0.00030210993,0.98420507,0.000035348752,0.000053612806,0.0017016657,0.0002631273,0.001196704,0.0030859355,0.0005192733,0.0085960785,0.000015649173],"about_ca_topic_score_codex":0.003375858,"about_ca_topic_score_gemma":0.008676088,"teacher_disagreement_score":0.003375858,"about_ca_system_score_codex":0.0002659984,"about_ca_system_score_gemma":0.00019213918,"threshold_uncertainty_score":0.0067124367},"labels":[],"label_agreement":null},{"id":"W2046466474","doi":"10.1088/0004-637x/765/1/28","title":"FAINT TIDAL FEATURES IN GALAXIES WITHIN THE CANADA-FRANCE-HAWAII TELESCOPE LEGACY SURVEY WIDE FIELDS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Redshift; Surface brightness; Elliptical galaxy","score_opus":0.005577412862434349,"score_gpt":0.19615324863997333,"score_spread":0.19057583577753898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046466474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99828005,0.00013190722,0.00005177837,0.000018745357,0.0000012203391,0.000003419361,0.0010194288,0.000009232108,0.0004843901],"genre_scores_gemma":[0.9977488,0.000081463615,0.00006869666,0.000011557623,0.0000040166688,0.000004019995,0.0018331998,0.0000029741427,0.00024526165],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954224,0.000035840185,0.000025031339,0.00011161729,0.00015622015,0.00012908172],"domain_scores_gemma":[0.99628973,0.0006195274,0.001210912,0.00035978464,0.0006369078,0.00088304543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048838474,0.00024948,0.00023201136,0.0032286625,0.0005723605,0.0009818943,0.00050109427,0.000310148,0.001743128],"category_scores_gemma":[0.0027543842,0.00017537129,0.00025296502,0.0022820833,0.00058718835,0.00040063707,0.0008907328,0.00020510974,0.00027229736],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000017473552,0.0000054567063,0.9974366,0.0000051359857,0.000024715348,0.00003782337,0.00022800342,0.000047699406,0.000431119,0.000022192484,0.00012494248,0.0016187528],"study_design_scores_gemma":[5.7316265e-7,0.0000036792858,0.99964416,0.0000015175461,0.000004290852,0.000025669944,0.00010020387,0.000040566185,0.00003100393,0.0000034430484,0.0001433662,0.0000014879813],"about_ca_topic_score_codex":0.31198174,"about_ca_topic_score_gemma":0.48951894,"teacher_disagreement_score":0.68801826,"about_ca_system_score_codex":0.0012823542,"about_ca_system_score_gemma":0.0005856133,"threshold_uncertainty_score":0.62033165},"labels":[],"label_agreement":null},{"id":"W2046507082","doi":"10.1086/312462","title":"The Magellanic Stream and the Density of Coronal Gas in the Galactic Halo","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Halo; Astrophysics; Galactic halo; Physics; Galaxy; Drag; Astronomy; Mechanics","score_opus":0.004929534082078212,"score_gpt":0.19705436280092484,"score_spread":0.19212482871884662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046507082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981116,0.00074694445,0.00009573676,0.000052434305,0.0000016605557,0.0000010151732,0.0000870839,0.000010978371,0.0008924507],"genre_scores_gemma":[0.9994561,0.0002648715,0.0000404448,0.000007660905,0.0000056874956,6.272157e-7,0.000076845376,0.0000023732175,0.00014532861],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999608,0.000007101958,0.0000020322434,0.000008252729,0.000008253664,0.000013630969],"domain_scores_gemma":[0.9995654,0.00010331691,0.0001186032,0.000026060996,0.000045910307,0.00014070328],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020335773,0.00013091815,0.00012773214,0.0007875673,0.00022702606,0.0008580241,0.0002149609,0.0002440338,0.0010587535],"category_scores_gemma":[0.0010905941,0.00015396118,0.000099082594,0.0006516774,0.000456471,0.00040391198,0.00037160006,0.00014061909,0.00021857109],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043717344,0.000044655415,0.94626904,0.00006966192,0.00012220243,0.00039467242,0.0006110244,0.006093662,0.02107055,0.00905132,0.00082442246,0.015011559],"study_design_scores_gemma":[0.000024102315,0.00004227007,0.98828083,0.000016375989,0.000037571623,0.00030249116,0.00034594763,0.0045304103,0.0018869116,0.003432144,0.0010858494,0.0000150457345],"about_ca_topic_score_codex":0.0098492885,"about_ca_topic_score_gemma":0.0071845273,"teacher_disagreement_score":0.0098492885,"about_ca_system_score_codex":0.0007008831,"about_ca_system_score_gemma":0.00014727173,"threshold_uncertainty_score":0.01958388},"labels":[],"label_agreement":null},{"id":"W2046509365","doi":"10.1088/0004-637x/702/1/368","title":"SHARPENING THE PRECISION OF THE SUNYAEV-ZEL'DOVICH POWER SPECTRUM","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"","keywords":"Cosmic microwave background; Sharpening; Physics; Spectral density; Masking (illustration); Sensitivity (control systems); Sample variance; Amplitude; Astrophysics; Noise (video); Variance (accounting); Sky; COSMIC cancer database; Gaussian; Computational physics; Statistical physics; Optics; Statistics; Mathematics; Computer science","score_opus":0.005906489557398281,"score_gpt":0.21265145503911712,"score_spread":0.20674496548171883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046509365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9303158,0.00015197076,0.06641418,0.00017935895,0.00002088814,0.000013074905,0.00023652926,0.00070800364,0.001960152],"genre_scores_gemma":[0.992159,0.000025229225,0.0075980974,0.00001330712,0.0000035832777,0.000004614308,0.00009905014,0.000038575778,0.000058508685],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9995254,0.00015643326,0.000022436905,0.000119961784,0.000111064335,0.00006470219],"domain_scores_gemma":[0.99612683,0.0023248105,0.00038479108,0.000829211,0.00021331981,0.000121128694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002382448,0.0005465645,0.00046364564,0.00058877346,0.0003309882,0.0011338822,0.0008575067,0.0005423871,0.0007851222],"category_scores_gemma":[0.009503098,0.000370654,0.0004914756,0.00046494132,0.00044206085,0.0006951265,0.00086920714,0.0005961441,0.0001545326],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053934543,0.00005502162,0.07334668,0.00011696611,0.0002487612,0.00016509819,0.0002935238,0.8693877,0.019336041,0.011319985,0.00072762836,0.024463234],"study_design_scores_gemma":[0.000057218356,0.000066698194,0.027392741,0.00002090386,0.000049970793,0.00007014097,0.00003155405,0.9556739,0.011522977,0.004580006,0.00048863643,0.00004531856],"about_ca_topic_score_codex":0.0060244836,"about_ca_topic_score_gemma":0.0046799607,"teacher_disagreement_score":0.0060244836,"about_ca_system_score_codex":0.000588226,"about_ca_system_score_gemma":0.0004917221,"threshold_uncertainty_score":0.012599707},"labels":[],"label_agreement":null},{"id":"W2046539265","doi":"10.1086/500401","title":"Angular Differential Imaging: A Powerful High‐Contrast Imaging Technique","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":989,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Speckle pattern; Telescope; Speckle noise; Noise (video); Field of view; Residual; Exoplanet; Angular resolution (graph drawing); Attenuation","score_opus":0.0033238303064010498,"score_gpt":0.1985493693571678,"score_spread":0.19522553905076676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046539265","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14077012,0.008918438,0.80817646,0.0006369767,0.0002908745,0.00022244875,0.0010362114,0.004724213,0.035224196],"genre_scores_gemma":[0.48095614,0.0038021747,0.4985949,0.00045649748,0.0002191425,0.00016007158,0.0014903765,0.0004507499,0.013869974],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99956864,0.00004737838,0.000015102456,0.000097942204,0.00020345682,0.00006746945],"domain_scores_gemma":[0.99963546,0.000078619865,0.000078754114,0.000083279905,0.000081356695,0.000042431413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046878183,0.00041139862,0.00040019237,0.0011441583,0.00030403247,0.0007399931,0.0010528765,0.0004738839,0.0033124543],"category_scores_gemma":[0.0004160606,0.0003541528,0.00027397939,0.0010982648,0.00037303648,0.00083351374,0.000954653,0.00080095284,0.0010205077],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016445354,0.000057181514,0.002239378,0.00039566815,0.000051462946,0.00026273087,0.000098094024,0.0009683185,0.87223434,0.0035945883,0.003881385,0.116052344],"study_design_scores_gemma":[0.0000624805,0.0002888138,0.009488686,0.00005418511,0.0000728062,0.0041078897,0.00007863028,0.032257862,0.8662673,0.0017085237,0.08551208,0.00010078569],"about_ca_topic_score_codex":0.0006776869,"about_ca_topic_score_gemma":0.0010053675,"teacher_disagreement_score":0.0033124543,"about_ca_system_score_codex":0.00041159298,"about_ca_system_score_gemma":0.00027580163,"threshold_uncertainty_score":0.011081338},"labels":[],"label_agreement":null},{"id":"W2046549947","doi":"10.1086/518232","title":"<i>K</i>‐Corrections and Spectral Templates of Type Ia Supernovae","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":367,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Victoria","funders":"","keywords":"Supernova; Physics; Spectral line; Broadband; Astrophysics; Rest frame; Rest (music); Spectral energy distribution; Range (aeronautics); Spectral shape analysis; Energy (signal processing); Frame (networking); Stellar classification; Computational physics; Optics; Galaxy; Computer science; Materials science; Astronomy; Redshift; Telecommunications","score_opus":0.01074557711743597,"score_gpt":0.24797864649335652,"score_spread":0.23723306937592054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046549947","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.85032827,0.00033442013,0.14122845,0.000116939416,0.000066239976,0.000057574274,0.001691685,0.0014149515,0.00476165],"genre_scores_gemma":[0.97073597,0.00015512401,0.025652247,0.000025127287,0.000016823216,0.000040238087,0.0019551588,0.00040250388,0.0010168786],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99914813,0.00017024175,0.00008828371,0.0002951844,0.00021631068,0.00008191223],"domain_scores_gemma":[0.9883908,0.0034212898,0.0034611435,0.0033189827,0.0011558185,0.00025200332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019354728,0.00039909116,0.00033768555,0.0011401479,0.0004299968,0.0013470395,0.0008266648,0.00040930984,0.0010609279],"category_scores_gemma":[0.029022418,0.0004162996,0.00062885624,0.0013492903,0.0003408426,0.00094177126,0.0005732376,0.00051087793,0.00070670125],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047800652,0.00010476514,0.57725537,0.00010466239,0.00029014825,0.00025032653,0.00027584913,0.2162696,0.038091157,0.012920063,0.0020230103,0.15193708],"study_design_scores_gemma":[0.00001398368,0.000075100106,0.6364505,0.000035572753,0.000120151635,0.00078461913,0.000084130836,0.30642277,0.04104991,0.010382225,0.00447739,0.00010358648],"about_ca_topic_score_codex":0.004016072,"about_ca_topic_score_gemma":0.0053326758,"teacher_disagreement_score":0.004016072,"about_ca_system_score_codex":0.0010345638,"about_ca_system_score_gemma":0.0005120724,"threshold_uncertainty_score":0.010235846},"labels":[],"label_agreement":null},{"id":"W2046575033","doi":"10.1088/0004-637x/729/1/62","title":"THE ATACAMA COSMOLOGY TELESCOPE: A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM AT 148 AND 218 GHz FROM THE 2008 SOUTHERN SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":178,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Cosmic microwave background; Physics; Astrophysics; Cosmology; Spectral density; Gravitational lens; Telescope; Astronomy; South Pole Telescope; Observational cosmology; Anisotropy; COSMIC cancer database; Galaxy; Dark energy; Redshift; Optics","score_opus":0.023861245169609396,"score_gpt":0.22307095250131478,"score_spread":0.1992097073317054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046575033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8978423,0.0005379416,0.004932312,0.00085755903,0.00011715911,0.00015790443,0.043140013,0.0006063178,0.051808562],"genre_scores_gemma":[0.9370626,0.00052303757,0.014644792,0.0004126194,0.00021116463,0.0001925342,0.035679992,0.00017896817,0.011094216],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996867,0.00004951781,0.000010839026,0.000072282746,0.0001417033,0.000038935388],"domain_scores_gemma":[0.99925905,0.000053801097,0.00017713611,0.00013323495,0.00021722532,0.00015952402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047338684,0.00018470247,0.00018230802,0.0014632514,0.00052670244,0.00045937925,0.00034143322,0.0002999084,0.0033566009],"category_scores_gemma":[0.001019076,0.00013887098,0.00011761914,0.00199792,0.00018799576,0.00041676633,0.0006145036,0.00043109385,0.0011894652],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003915903,0.00020960957,0.8039899,0.00017940796,0.00018672635,0.00028794943,0.0019384229,0.00034648043,0.03964388,0.003206811,0.05283362,0.096785635],"study_design_scores_gemma":[0.000030436937,0.00003560183,0.9610921,0.000013370961,0.000023328133,0.0001640897,0.00023374333,0.0002560908,0.0014705807,0.00028072132,0.036388356,0.000011609095],"about_ca_topic_score_codex":0.016828544,"about_ca_topic_score_gemma":0.045027558,"teacher_disagreement_score":0.016828544,"about_ca_system_score_codex":0.000334518,"about_ca_system_score_gemma":0.0005066277,"threshold_uncertainty_score":0.033461154},"labels":[],"label_agreement":null},{"id":"W2046730664","doi":"10.1088/0004-637x/799/1/7","title":"VERITAS OBSERVATIONS OF THE BL LAC OBJECT PG 1553+113","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Crab Nebula; BL Lac object; Extragalactic background light; Redshift; Opacity; Flux (metallurgy); Cutoff; Light curve; Power law","score_opus":0.02675996623575245,"score_gpt":0.23390121871759748,"score_spread":0.20714125248184503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046730664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99119616,0.00048541286,0.0005537742,0.00006119488,0.00001769368,0.00001638784,0.0028761462,0.00020852694,0.004584688],"genre_scores_gemma":[0.9895034,0.00021941116,0.0013546882,0.00006580985,0.00004827377,0.000017154907,0.0075917747,0.000050927585,0.0011486778],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997372,0.000015089309,0.000009530549,0.00008819468,0.000080367514,0.000069591435],"domain_scores_gemma":[0.9994492,0.000043034328,0.0002547703,0.00006192377,0.000052275445,0.00013885426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036009794,0.00042969768,0.0003132474,0.001259179,0.00045729606,0.00079359976,0.00044396354,0.0003775373,0.0017718062],"category_scores_gemma":[0.00045613802,0.0002351069,0.0003982368,0.0010806533,0.00043676508,0.00033696534,0.00083339826,0.00040851915,0.0006384949],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015021309,0.00017351678,0.8186128,0.0002631022,0.00046829827,0.0014786783,0.0010600511,0.0035807213,0.10661064,0.0016231555,0.00829992,0.056326944],"study_design_scores_gemma":[0.00003803862,0.00013339696,0.9882234,0.000021387523,0.000077001365,0.00043546618,0.00013065088,0.0011631844,0.002740776,0.00016748474,0.0068457834,0.000023424369],"about_ca_topic_score_codex":0.017391661,"about_ca_topic_score_gemma":0.036757994,"teacher_disagreement_score":0.017391661,"about_ca_system_score_codex":0.0012764789,"about_ca_system_score_gemma":0.00036955686,"threshold_uncertainty_score":0.034580827},"labels":[],"label_agreement":null},{"id":"W2046780919","doi":"10.1088/0004-637x/759/2/139","title":"GOODS-<i>HERSCHEL</i>: IMPACT OF ACTIVE GALACTIC NUCLEI AND STAR FORMATION ACTIVITY ON INFRARED SPECTRAL ENERGY DISTRIBUTIONS AT HIGH REDSHIFT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":175,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Active galactic nucleus; Spectral energy distribution; Galaxy; Star formation; Redshift; Infrared; Black-body radiation; Astronomy; Luminous infrared galaxy; Optics","score_opus":0.007773953893127424,"score_gpt":0.22379889046054288,"score_spread":0.21602493656741545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046780919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99310726,0.0001196322,0.00039384878,0.00008492988,0.0000021088113,0.0000035302135,0.004683031,0.000099961115,0.0015056601],"genre_scores_gemma":[0.98940736,0.000053031417,0.00089113635,0.00004984374,0.0000051649604,0.0000030336435,0.008542242,0.000046889774,0.0010013618],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997714,0.000050890394,0.000011230116,0.00007040618,0.000047591795,0.00004856083],"domain_scores_gemma":[0.99917537,0.00026808126,0.0002446587,0.00013087908,0.000061871324,0.00011915779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005267391,0.0001875993,0.00017940786,0.0006130286,0.00015639907,0.00068366784,0.00028995314,0.0001992574,0.00242686],"category_scores_gemma":[0.0009584748,0.00010517603,0.0003847076,0.0007172515,0.00025410866,0.00033734302,0.00040462826,0.0002154361,0.00058452203],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000119910605,0.00002555663,0.9794804,0.000030483665,0.00015349545,0.00008189672,0.00007960285,0.006722778,0.004498327,0.00037610068,0.0015246676,0.0069067357],"study_design_scores_gemma":[0.000004094064,0.000016848127,0.99355984,0.0000027766494,0.000017210405,0.00003154,0.000045170735,0.0036656617,0.0016160574,0.00006404927,0.00097102165,0.0000057811367],"about_ca_topic_score_codex":0.03597052,"about_ca_topic_score_gemma":0.06630575,"teacher_disagreement_score":0.03597052,"about_ca_system_score_codex":0.0005167043,"about_ca_system_score_gemma":0.000191666,"threshold_uncertainty_score":0.071522295},"labels":[],"label_agreement":null},{"id":"W2046831843","doi":"10.1088/0004-637x/726/1/31","title":"THE ACS FORNAX CLUSTER SURVEY. IV. DEPROJECTION OF THE SURFACE BRIGHTNESS PROFILES OF EARLY-TYPE GALAXIES IN THE VIRGO AND FORNAX CLUSTERS: INVESTIGATING THE “CORE/POWER-LAW DICHOTOMY”","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Surface brightness; Fornax Cluster; Virgo Cluster; Galaxy; Luminosity; Luminosity function; Extrapolation; Advanced Camera for Surveys; Surface brightness fluctuation","score_opus":0.012835738401013997,"score_gpt":0.23386411349406205,"score_spread":0.22102837509304807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046831843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95782924,0.0004329728,0.0009757927,0.0002463041,0.000027662954,0.00006060947,0.027155448,0.00037040166,0.012901599],"genre_scores_gemma":[0.96631014,0.00018052719,0.0036988524,0.00011950556,0.000027195889,0.00006163023,0.025676522,0.000053064017,0.0038725398],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984396,0.00001744208,0.0000061310266,0.000054997257,0.000054358487,0.00002310685],"domain_scores_gemma":[0.99965346,0.000024009712,0.0001299035,0.000073375675,0.000060152044,0.00005906735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000319843,0.0002689363,0.00020440418,0.0015034798,0.00028762635,0.00038946758,0.00039047858,0.00022341637,0.0016085589],"category_scores_gemma":[0.000665788,0.000074629424,0.00025592736,0.0010211378,0.00017146001,0.00029528237,0.00038269264,0.0002173143,0.0010796845],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026718056,0.0000733718,0.9240968,0.00007101713,0.00014556588,0.0001898738,0.0006078024,0.0014954213,0.010891838,0.0017425063,0.019827899,0.04059079],"study_design_scores_gemma":[0.000007205318,0.000014502283,0.9932181,0.000005260961,0.00000785361,0.000051759882,0.000072798415,0.0007203027,0.00042278034,0.00010716882,0.0053669894,0.0000052130754],"about_ca_topic_score_codex":0.03089079,"about_ca_topic_score_gemma":0.04589062,"teacher_disagreement_score":0.03089079,"about_ca_system_score_codex":0.00057508505,"about_ca_system_score_gemma":0.00026680023,"threshold_uncertainty_score":0.06142199},"labels":[],"label_agreement":null},{"id":"W2046900054","doi":"10.1088/0004-637x/739/1/13","title":"AN ASTEROSEISMIC MEMBERSHIP STUDY OF THE RED GIANTS IN THREE OPEN CLUSTERS OBSERVED BY<i>KEPLER</i>: NGC 6791, NGC 6819, AND NGC 6811","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Asteroseismology; Astrophysics; Stars; Open cluster; Photometry (optics); Kepler; Astronomy; Star cluster; Blue straggler; Red clump; Milky Way","score_opus":0.05728082762986942,"score_gpt":0.25072504027901554,"score_spread":0.19344421264914613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046900054","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996977,0.000009692204,0.000014557246,0.00000743629,5.054295e-7,9.679295e-7,0.000059787984,8.3149047e-7,0.00020849875],"genre_scores_gemma":[0.999271,0.000014076723,0.00003284772,0.000007044637,0.0000021088028,0.0000017534236,0.0002887562,0.0000017541444,0.0003806093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998988,0.000012374407,0.0000061363876,0.000031541917,0.00001679637,0.000034354605],"domain_scores_gemma":[0.99938655,0.000084144885,0.00015225892,0.000035632995,0.00011515829,0.00022613718],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017965179,0.00015561956,0.00017500446,0.0015470138,0.00089231244,0.0004386701,0.00023003054,0.00033386168,0.0019135716],"category_scores_gemma":[0.0004473233,0.00013710091,0.00014183742,0.0011131671,0.00036632002,0.00033157974,0.00070270797,0.00022419308,0.0003842027],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015960602,0.00006193843,0.9884077,0.000008294757,0.000018103943,0.00019515022,0.0021377513,0.00005963353,0.005988326,0.000098575845,0.00020840346,0.002656579],"study_design_scores_gemma":[0.000002275916,0.0000149073785,0.99866474,0.0000013688307,0.0000066819953,0.00008574089,0.0008829374,0.0000511304,0.0001155005,0.000014200308,0.00015922463,0.0000013848921],"about_ca_topic_score_codex":0.020500956,"about_ca_topic_score_gemma":0.041190557,"teacher_disagreement_score":0.020500956,"about_ca_system_score_codex":0.00033070968,"about_ca_system_score_gemma":0.0002162115,"threshold_uncertainty_score":0.04076326},"labels":[],"label_agreement":null},{"id":"W2046906152","doi":"10.1086/308979","title":"The MACHO Project Sample of Galactic Bulge High‐Amplitude δ Scuti Stars: Pulsation Behavior and Stellar Properties","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Bulge; Stars; Light curve; Photometry (optics); Astronomy; Red clump; Population; Amplitude; Gravitational microlensing; Milky Way","score_opus":0.018520614868458945,"score_gpt":0.23724239742770528,"score_spread":0.21872178255924635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046906152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.969409,0.00041277567,0.00047704962,0.00013420316,0.000011448028,0.000105350635,0.022982273,0.00014021795,0.0063277753],"genre_scores_gemma":[0.9126729,0.00037719737,0.0019389801,0.00018380773,0.00006810655,0.00022927593,0.07556599,0.00008768219,0.008876002],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984205,0.000023406868,0.000014141419,0.000038686176,0.000052013525,0.00002963178],"domain_scores_gemma":[0.9994836,0.000027350765,0.0001196953,0.00011635371,0.00010583754,0.00014709581],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003593829,0.00023359798,0.00029058053,0.001456147,0.00044823613,0.00064353074,0.0004589098,0.00027232437,0.0023777052],"category_scores_gemma":[0.0009768626,0.00016887739,0.00018393814,0.0011982888,0.00023243074,0.00035397624,0.0015447793,0.00018724868,0.0013473205],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006651164,0.0002277066,0.93743753,0.00008982224,0.00010678217,0.00023796452,0.0007112185,0.00015948171,0.0057594366,0.0005737229,0.016618535,0.037412785],"study_design_scores_gemma":[0.000044579578,0.00005513733,0.983206,0.000011942675,0.000028828534,0.00033388182,0.00037085442,0.0003074709,0.00054074207,0.00010462558,0.014990111,0.000005881702],"about_ca_topic_score_codex":0.008045808,"about_ca_topic_score_gemma":0.014405037,"teacher_disagreement_score":0.008045808,"about_ca_system_score_codex":0.00026388414,"about_ca_system_score_gemma":0.00033104312,"threshold_uncertainty_score":0.015998006},"labels":[],"label_agreement":null},{"id":"W2046919095","doi":"10.1086/512803","title":"Molecular and Atomic Excitation Stratification in the Outflow of the Planetary Nebula M27","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Ionization; Orion Nebula; Planetary nebula; Outflow; Dissociation (chemistry); Spectroscopy; Dissociative recombination; Nebula; Balmer series; Photon","score_opus":0.007525435371921023,"score_gpt":0.22865467728184075,"score_spread":0.22112924190991973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046919095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99830186,0.000079818594,0.00014562694,0.000044955286,0.0000018039707,0.0000027975345,0.00021567018,0.000025670484,0.0011817778],"genre_scores_gemma":[0.99877626,0.00008411195,0.00027673092,0.000022999731,0.000004477104,0.000005996892,0.00039118397,0.000013804768,0.00042429182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999541,0.0000024706717,0.0000019088122,0.000015266822,0.000010942486,0.000015333619],"domain_scores_gemma":[0.999902,0.000009566509,0.000029236046,0.000009219503,0.000017643004,0.00003233402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010676196,0.0002356599,0.0002131386,0.000767273,0.00035135972,0.0004186781,0.0002574955,0.00024604207,0.0011321402],"category_scores_gemma":[0.00030903023,0.00016729042,0.00017982934,0.00037990065,0.00025493957,0.00026952953,0.00046920386,0.00025938964,0.0003883046],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002499503,0.00007808854,0.83646816,0.000047173624,0.00008454164,0.0011146968,0.0009828781,0.0022458837,0.14209257,0.0011385445,0.0012557895,0.014241623],"study_design_scores_gemma":[0.000012058234,0.00003127662,0.9933664,0.00000798038,0.000014040909,0.00023226313,0.00033112426,0.002448366,0.001950477,0.00017170345,0.0014268123,0.000007512017],"about_ca_topic_score_codex":0.007590074,"about_ca_topic_score_gemma":0.007871539,"teacher_disagreement_score":0.007590074,"about_ca_system_score_codex":0.0005681707,"about_ca_system_score_gemma":0.0002582811,"threshold_uncertainty_score":0.015091836},"labels":[],"label_agreement":null},{"id":"W2046931470","doi":"10.1086/587678","title":"Galaxy Clusters in the Line of Sight to Background Quasars. I. Survey Design and Incidence of Mg<scp>ii</scp>Absorbers at Cluster Redshifts","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Redshift; Quasar; Astrophysics; Physics; Cluster (spacecraft); Galaxy; Population; Galaxy cluster; Equivalent width; Astronomy; Spectral line; Emission spectrum; Demography","score_opus":0.02423744940155549,"score_gpt":0.23960955772860812,"score_spread":0.2153721083270526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2046931470","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99674773,0.000113262446,0.00013025354,0.000030266854,0.0000018484974,0.00001380019,0.0016395455,0.000010935979,0.0013122307],"genre_scores_gemma":[0.99773884,0.0000686847,0.0001810756,0.000015026152,0.0000029443142,0.00001301765,0.0013901241,0.0000024191913,0.0005878322],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995827,0.00008096541,0.000026922879,0.00012508387,0.000085659114,0.00009859285],"domain_scores_gemma":[0.9977648,0.00026207694,0.0008237016,0.0001350748,0.00043056248,0.0005838246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042218537,0.000118432945,0.0001224412,0.0021048058,0.00043396727,0.00048546024,0.00034158115,0.00022487943,0.0017306744],"category_scores_gemma":[0.0019480842,0.0001611853,0.00013394059,0.0018520181,0.00029938304,0.00040484525,0.0008667368,0.00013816987,0.0004550295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005132125,0.0000103950415,0.99636227,0.0000066081207,0.0000090040985,0.000013061552,0.00016186532,0.000058487814,0.0003830711,0.000068358706,0.00023438694,0.0026412022],"study_design_scores_gemma":[8.6634276e-7,0.000017480179,0.9994005,0.0000014086075,0.000003973393,0.000020870239,0.00022794509,0.00005238878,0.000047692203,0.000011092233,0.00021490094,9.1067875e-7],"about_ca_topic_score_codex":0.07021109,"about_ca_topic_score_gemma":0.15246563,"teacher_disagreement_score":0.07021109,"about_ca_system_score_codex":0.0006122391,"about_ca_system_score_gemma":0.00054915954,"threshold_uncertainty_score":0.1396048},"labels":[],"label_agreement":null},{"id":"W2047043448","doi":"10.1088/0004-637x/758/1/34","title":"NEUTRINO PROCESSES IN PARTIALLY DEGENERATE NEUTRON MATTER","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Carleton University; TRIUMF","funders":"Natural Sciences and Engineering Research Council of Canada; Emberi Eroforrások Minisztériuma; European Social Fund; Deutsche Forschungsgemeinschaft","keywords":"Physics; Neutrino; Supernova; Degenerate energy levels; Spin (aerodynamics); Neutron; Neutron star; Nuclear physics; Particle physics; Astrophysics; Quantum mechanics","score_opus":0.019989008653581407,"score_gpt":0.28228152819383956,"score_spread":0.2622925195402582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047043448","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936056,0.00014977876,0.0028130896,0.00010647658,0.000016074791,0.000020209125,0.00011108046,0.00005740432,0.0031201842],"genre_scores_gemma":[0.99841344,0.00006668656,0.0011048641,0.000024472723,0.0000064442884,0.000010960902,0.0001037099,0.000019574612,0.00024988496],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99976736,0.00006964214,0.000011785659,0.000023539475,0.00004850685,0.00007915268],"domain_scores_gemma":[0.99889416,0.0004502357,0.00022874682,0.00009527387,0.00013123453,0.00020038451],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071944867,0.00057986454,0.00072415196,0.00075574324,0.001008847,0.00081569824,0.00084607094,0.00077700167,0.0011438766],"category_scores_gemma":[0.004109338,0.0003552154,0.0006321926,0.0005292605,0.0010471132,0.0009152819,0.0013714796,0.00080797233,0.000099649405],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050902524,0.00022743025,0.020516997,0.00009766683,0.00013960007,0.0006615187,0.0003335639,0.9360213,0.012230794,0.02593153,0.00039330035,0.0029372973],"study_design_scores_gemma":[0.000072447634,0.00012703998,0.0035990886,0.00001554532,0.00002064332,0.00006823217,0.00010844938,0.98406625,0.003741411,0.0077965576,0.00035379027,0.000030602274],"about_ca_topic_score_codex":0.007990829,"about_ca_topic_score_gemma":0.00489962,"teacher_disagreement_score":0.007990829,"about_ca_system_score_codex":0.0008728602,"about_ca_system_score_gemma":0.0006820133,"threshold_uncertainty_score":0.015888631},"labels":[],"label_agreement":null},{"id":"W2047128407","doi":"10.1088/0004-637x/705/1/237","title":"STRUCTURAL PARAMETERS OF THE MESSIER 87 GLOBULAR CLUSTERS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Milky Way; Virgo Cluster; Cluster (spacecraft); Star cluster; Hubble space telescope; Advanced Camera for Surveys; Galaxy; Galaxy cluster; Open cluster; Elliptical galaxy; Astronomy; Stars","score_opus":0.006819181561776454,"score_gpt":0.20972163392674148,"score_spread":0.202902452364965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047128407","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99596846,0.0001263223,0.000745801,0.000034205113,0.0000016179223,0.000005398328,0.0006515391,0.000050510294,0.00241618],"genre_scores_gemma":[0.99747795,0.000063802116,0.00071779575,0.0000108141485,0.0000030538915,0.000005685422,0.0011130236,0.000015548201,0.0005923077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999409,0.0000047337276,0.0000037770812,0.00002176182,0.0000152416105,0.000013560177],"domain_scores_gemma":[0.99982506,0.00003414731,0.000050475737,0.000030545558,0.00003089678,0.000029036464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015390087,0.00018480411,0.0001358927,0.0011932071,0.00025394713,0.00036471212,0.00027504354,0.00019569298,0.0014320129],"category_scores_gemma":[0.0007944726,0.00013823576,0.00020243516,0.0004979866,0.0001585556,0.00019067712,0.00033646985,0.00014893957,0.00059455953],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022036294,0.000023431585,0.8626617,0.0000758284,0.00013567934,0.00034098953,0.00097381615,0.055706676,0.026387878,0.008183132,0.0037612892,0.04152921],"study_design_scores_gemma":[0.000014066896,0.000021217218,0.9483307,0.00001431511,0.00003655317,0.00016783857,0.00017309452,0.040385433,0.0043798178,0.0020378062,0.0044191857,0.00001998415],"about_ca_topic_score_codex":0.007883126,"about_ca_topic_score_gemma":0.008172926,"teacher_disagreement_score":0.007883126,"about_ca_system_score_codex":0.0006826606,"about_ca_system_score_gemma":0.00015943432,"threshold_uncertainty_score":0.015674472},"labels":[],"label_agreement":null},{"id":"W2047206943","doi":"10.1086/503533","title":"Measurement of Ω<sub><i>m</i></sub>, Ω<sub>Λ</sub>from a Blind Analysis of Type Ia Supernovae with CMAGIC: Using Color Information to Verify the Acceleration of the Universe","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Supernova; Luminosity; Redshift; Cosmology; Galaxy; Magnitude (astronomy); Acceleration; Universe; Light curve; Absolute magnitude; Shape of the universe; Dark energy; Type (biology); Cosmological constant; Theoretical physics","score_opus":0.015460726569381824,"score_gpt":0.22056979090745643,"score_spread":0.2051090643380746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047206943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92896605,0.0009438672,0.037186872,0.00035554045,0.00046771628,0.00010818987,0.010253505,0.0021414766,0.019576706],"genre_scores_gemma":[0.9533834,0.0004154397,0.03344522,0.00023473172,0.0001246445,0.000058834343,0.0049344897,0.000475128,0.006928137],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9996766,0.00002907715,0.000028305421,0.00011503988,0.00010854924,0.000042370924],"domain_scores_gemma":[0.9988544,0.0001491562,0.0002278114,0.0002497532,0.00028468767,0.00023417501],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004546835,0.00040264602,0.00028464303,0.0017580321,0.00039551806,0.00074422325,0.00042167134,0.000650147,0.0063816896],"category_scores_gemma":[0.001301357,0.00035900174,0.00042854412,0.0010663926,0.00025237602,0.0005413404,0.00069914624,0.0005028939,0.0033092361],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00247581,0.00017656731,0.17179663,0.00036083817,0.00033021093,0.000504782,0.00033447586,0.00045044458,0.7135653,0.0020341533,0.008838824,0.09913201],"study_design_scores_gemma":[0.00006551794,0.00022537274,0.7515984,0.00004234378,0.00029866392,0.0013554591,0.00013780188,0.002395508,0.23076415,0.0013060259,0.01171963,0.00009106854],"about_ca_topic_score_codex":0.0011131136,"about_ca_topic_score_gemma":0.002144565,"teacher_disagreement_score":0.0063816896,"about_ca_system_score_codex":0.00023222914,"about_ca_system_score_gemma":0.00023260542,"threshold_uncertainty_score":0.021348894},"labels":[],"label_agreement":null},{"id":"W2047272174","doi":"10.1086/588725","title":"On the Constancy of the Characteristic Mass of Young Stars","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Physics; Metallicity; Stars; Star formation; Redshift; Molecular cloud; Initial mass function; Thermal; Ionization; Fragmentation (computing); Galaxy; Thermodynamics; Ion","score_opus":0.011800605765412498,"score_gpt":0.21354282714696882,"score_spread":0.2017422213815563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047272174","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95241755,0.0020378463,0.026744904,0.0004915755,0.000046319743,0.000008831834,0.00032089153,0.00026905714,0.01766303],"genre_scores_gemma":[0.99633044,0.00032173007,0.002272791,0.000051180952,0.00002415962,0.000007894496,0.00010039894,0.000037135036,0.00085432496],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979824,0.000024027164,0.000010240362,0.00010004332,0.000037758353,0.000029660025],"domain_scores_gemma":[0.9980318,0.00076343043,0.00062538276,0.00024985924,0.00018762413,0.00014190802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049579865,0.00016691248,0.00017987238,0.00052674086,0.00026987202,0.00077397656,0.00046930273,0.00041595806,0.00095364073],"category_scores_gemma":[0.005637892,0.00023527801,0.00022253492,0.0003559286,0.0007619634,0.0010134064,0.0004702606,0.00034919832,0.00042693372],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047186678,0.000060764138,0.55869174,0.0003223997,0.00015893891,0.0011243935,0.0010978143,0.060059085,0.09211055,0.16933584,0.0031631081,0.11340349],"study_design_scores_gemma":[0.000047164896,0.00017093278,0.7552169,0.00011798022,0.000060352726,0.0021426845,0.00023293126,0.12765901,0.02359163,0.07525951,0.015387886,0.00011301576],"about_ca_topic_score_codex":0.0012281138,"about_ca_topic_score_gemma":0.0007797527,"teacher_disagreement_score":0.0012281138,"about_ca_system_score_codex":0.0005096736,"about_ca_system_score_gemma":0.00025933003,"threshold_uncertainty_score":0.0036979914},"labels":[],"label_agreement":null},{"id":"W2047340280","doi":"10.1086/587160","title":"Additional Ultracool White Dwarfs Found in the Sloan Digital Sky Survey","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"White dwarf; Balmer series; Physics; Astrophysics; Sky; Photometry (optics); Stars; Astronomy; Stellar classification; Spectral line; Proper motion; Emission spectrum","score_opus":0.018082009042425955,"score_gpt":0.22024233129741866,"score_spread":0.2021603222549927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047340280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978417,0.00024463315,0.00020039,0.000034929923,0.000006606053,0.0000041709254,0.00043855922,0.000018729139,0.0012101977],"genre_scores_gemma":[0.995415,0.00022039363,0.00078341784,0.000041284162,0.00001617715,0.0000070022647,0.002473918,0.000007568467,0.0010352867],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958414,0.000023079047,0.000038774735,0.00009104979,0.0001673273,0.00009572798],"domain_scores_gemma":[0.9988745,0.00012534045,0.00042328672,0.00014838116,0.0001257372,0.00030269005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039568738,0.00023141112,0.0002623426,0.0019528721,0.00058236805,0.0006069815,0.00022447993,0.00015738388,0.00069360377],"category_scores_gemma":[0.0007484715,0.00011905559,0.00018326765,0.001455431,0.0003529002,0.00035924243,0.0009186718,0.00022352673,0.00023940913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001305897,0.00004926183,0.9572708,0.000060868886,0.00005712832,0.0017182562,0.0010010717,0.00015169762,0.012395277,0.0006617102,0.0010560394,0.025447417],"study_design_scores_gemma":[0.000013173474,0.00007313912,0.9799715,0.000014291627,0.00003688129,0.0025071516,0.00053879974,0.0003287162,0.0021024467,0.00031848723,0.0140816225,0.000013754797],"about_ca_topic_score_codex":0.010843471,"about_ca_topic_score_gemma":0.0311892,"teacher_disagreement_score":0.010843471,"about_ca_system_score_codex":0.00048821908,"about_ca_system_score_gemma":0.0004769594,"threshold_uncertainty_score":0.021560669},"labels":[],"label_agreement":null},{"id":"W2047352035","doi":"10.1086/512002","title":"Astrometric Perturbations in Substructure Lensing","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Waterloo; University of Toronto","funders":"","keywords":"Substructure; Physics; Gravitational lens; Observable; Einstein radius; Lens (geology); Galaxy; Strong gravitational lensing; Astrophysics; RADIUS; Halo; Optics; Computer science","score_opus":0.00811408059869468,"score_gpt":0.21832014498275257,"score_spread":0.2102060643840579,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047352035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9136956,0.00063752255,0.074094996,0.0005506369,0.000032742148,0.00003150169,0.00015522425,0.00039895676,0.010402865],"genre_scores_gemma":[0.9964395,0.000082502615,0.0028879794,0.000020376416,0.000009252106,0.000006310767,0.000033230626,0.000025006311,0.0004958635],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997062,0.00009056137,0.000011221055,0.000049191367,0.00010239238,0.000040420906],"domain_scores_gemma":[0.9986706,0.0005855065,0.00039366295,0.00012077575,0.00011922555,0.000110325986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069877255,0.0005350592,0.00035915477,0.00073586626,0.0005571515,0.0008421363,0.0005479765,0.0005657201,0.0011186241],"category_scores_gemma":[0.0071391882,0.00035302626,0.0004035448,0.0005750067,0.0011931004,0.0013847735,0.00089198985,0.00051573396,0.00011629201],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000071774986,0.000019638666,0.013330575,0.000024506415,0.000031908876,0.0001332004,0.00009649836,0.93733215,0.0043357457,0.04027691,0.00024100114,0.00410609],"study_design_scores_gemma":[0.000012021942,0.000018213874,0.0045016967,0.0000044179887,0.0000051019047,0.000041436222,0.000021574957,0.97976214,0.0009581844,0.014392027,0.00026935965,0.00001380734],"about_ca_topic_score_codex":0.013117332,"about_ca_topic_score_gemma":0.004528836,"teacher_disagreement_score":0.013117332,"about_ca_system_score_codex":0.0016992771,"about_ca_system_score_gemma":0.00049698557,"threshold_uncertainty_score":0.02608198},"labels":[],"label_agreement":null},{"id":"W2047373155","doi":"10.1088/0004-637x/775/2/135","title":"<i>SWIFT</i>OBSERVATIONS OF 1FGL J1018.6–5856","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Swift; Flux (metallurgy); Phase (matter); X-ray; Telescope; Gamma ray; Spectral line; Astronomy; Optics; Materials science","score_opus":0.017081055821725113,"score_gpt":0.2226797088327048,"score_spread":0.20559865301097968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047373155","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99563134,0.00029711897,0.00018854592,0.00008656737,0.000023695358,0.000010491914,0.001133124,0.00007681193,0.002552254],"genre_scores_gemma":[0.9901232,0.00017521478,0.0017961148,0.00014996492,0.00006633806,0.000016662974,0.006180216,0.000028650828,0.0014635519],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998087,0.000007330352,0.000014689458,0.000056674864,0.0000589774,0.000053626452],"domain_scores_gemma":[0.9994987,0.000027591343,0.0002781802,0.000044272863,0.00004356175,0.00010760055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003031141,0.00036060758,0.0005514081,0.0015361082,0.00066028035,0.00073809363,0.000584094,0.0005807547,0.001487907],"category_scores_gemma":[0.00045328378,0.00024919782,0.00022623173,0.0009261911,0.00028541533,0.0004084613,0.0006226039,0.00045319696,0.0010674843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077738083,0.00061836827,0.7242999,0.00026859835,0.00017609492,0.0033106084,0.00068723934,0.0015250867,0.2152893,0.00044953177,0.0060470584,0.04655091],"study_design_scores_gemma":[0.00003226217,0.00015652539,0.9898822,0.000019269804,0.00002527447,0.00090340484,0.000088920075,0.0009032154,0.003901367,0.00006618348,0.0040019825,0.000019364606],"about_ca_topic_score_codex":0.005219175,"about_ca_topic_score_gemma":0.015547509,"teacher_disagreement_score":0.005219175,"about_ca_system_score_codex":0.0004874485,"about_ca_system_score_gemma":0.00020655183,"threshold_uncertainty_score":0.010377586},"labels":[],"label_agreement":null},{"id":"W2047529987","doi":"10.1086/593202","title":"Gamma Rays from Ultra-High-Energy Cosmic Rays in Cygnus A","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Concordia University","funders":"","keywords":"Physics; Cosmic ray; Fermi Gamma-ray Space Telescope; Astrophysics; Gamma ray; Astronomy; Ultra-high-energy cosmic ray; Halo; Synchrotron; Galaxy; Active galactic nucleus; Spitzer Space Telescope; Telescope; Electron; Nuclear physics","score_opus":0.008392896805260935,"score_gpt":0.19481493647044543,"score_spread":0.1864220396651845,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047529987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9818626,0.0017640233,0.001304676,0.00021330602,0.00002470897,0.000036990892,0.0002474891,0.00010115424,0.014444981],"genre_scores_gemma":[0.99780804,0.000363517,0.00036409506,0.00006391684,0.000014365466,0.000015450098,0.00023725897,0.000019693154,0.001113537],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999018,0.000018885568,0.0000047876138,0.000022163516,0.000024160401,0.000028193728],"domain_scores_gemma":[0.9996203,0.00010693046,0.00014628268,0.000022931197,0.000034339864,0.000069102076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002864253,0.00090386055,0.0003944498,0.0013065707,0.00063820987,0.0012312885,0.0005019296,0.00070992776,0.0040120594],"category_scores_gemma":[0.00086519006,0.0003216683,0.0004975966,0.0012290874,0.0007402022,0.00052870053,0.0011341689,0.0005422511,0.0004540174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019562948,0.0005036981,0.6673473,0.000880842,0.0005087667,0.0148167405,0.0016285892,0.079514086,0.118030034,0.07723707,0.004447997,0.033128556],"study_design_scores_gemma":[0.0004406969,0.00034339036,0.88261604,0.00023109556,0.0003293947,0.0031833863,0.00048539665,0.05834197,0.010023845,0.040663928,0.0032452396,0.00009564655],"about_ca_topic_score_codex":0.010732621,"about_ca_topic_score_gemma":0.009102065,"teacher_disagreement_score":0.010732621,"about_ca_system_score_codex":0.0012237261,"about_ca_system_score_gemma":0.0004215347,"threshold_uncertainty_score":0.02134031},"labels":[],"label_agreement":null},{"id":"W2047542085","doi":"10.1086/589234","title":"The Peculiar Magnetic Field Morphology of the White Dwarf WD 1953−011: Evidence for a Large‐Scale Magnetic Flux Tube?","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Royal Military College of Canada","funders":"Science and Technology Facilities Council","keywords":"Physics; Magnetic field; Dipole; Photosphere; Astrophysics; Field strength; Rotation period; L-shell; Field line; Magnetic flux; Flux tube; Superposition principle; Quadrupole; Rotation (mathematics); White dwarf; Magnetic dipole; Field (mathematics); Geometry; Atomic physics; Stars; Earth's magnetic field","score_opus":0.016617593283479025,"score_gpt":0.23986535642316187,"score_spread":0.22324776313968284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047542085","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881965,0.00018185597,0.0002491788,0.000030135356,0.0000037623113,0.00000255502,0.000054119577,0.000012869417,0.0006458535],"genre_scores_gemma":[0.9996582,0.000047622005,0.00013948273,0.00000832932,0.0000051113147,0.000001224837,0.000046225723,0.0000015257813,0.00009223731],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999752,0.000001733934,0.000002015108,0.000011592784,0.0000042030993,0.0000052264886],"domain_scores_gemma":[0.9999361,0.0000058175115,0.000029898029,0.000008661521,0.0000051354777,0.000014382162],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000056050485,0.00013117932,0.0001234911,0.00032277175,0.0001771526,0.0004078514,0.00018161541,0.00021016726,0.0004885952],"category_scores_gemma":[0.00017935364,0.00008412686,0.00009509618,0.00027607288,0.00035251505,0.00016363313,0.00020936942,0.00007777433,0.0001654654],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039670517,0.00005443578,0.66140497,0.00013816105,0.000058786747,0.0022151656,0.0005837732,0.0011094155,0.3044184,0.0014395263,0.0005266066,0.02765402],"study_design_scores_gemma":[0.000014630594,0.000048768554,0.99175733,0.0000092343025,0.000020002153,0.00095222396,0.0001780394,0.0011309806,0.0043839663,0.00035306235,0.0011389278,0.000012797117],"about_ca_topic_score_codex":0.0040755128,"about_ca_topic_score_gemma":0.0049884357,"teacher_disagreement_score":0.0040755128,"about_ca_system_score_codex":0.0003384089,"about_ca_system_score_gemma":0.000098652876,"threshold_uncertainty_score":0.008103609},"labels":[],"label_agreement":null},{"id":"W2047577395","doi":"10.1086/432441","title":"X-Ray Timing, Spectroscopy, and Photometry of the Anomalous X-Ray Pulsar Candidate CXOU J010043.1-721134","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Astrophysics; Magnetar; Neutron star; X-ray pulsar; Observatory; Photometry (optics); Astronomy; Black-body radiation; Stars; Radiation","score_opus":0.008887551674552456,"score_gpt":0.29714484376812833,"score_spread":0.28825729209357587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047577395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988959,0.00005455726,0.00009118428,0.00002126058,0.000004910537,0.000005071209,0.00024412539,0.0000119094075,0.00067109644],"genre_scores_gemma":[0.9975821,0.000052479107,0.00051879004,0.000021120046,0.000012937171,0.000009140582,0.0013141768,0.000009422078,0.00047987953],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989605,0.000009383272,0.0000081411945,0.000019167173,0.000033443735,0.000033774995],"domain_scores_gemma":[0.99961734,0.000035030545,0.00017497125,0.000024599844,0.000054335804,0.000093735514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001519678,0.00018993081,0.00029180042,0.000997751,0.00054054795,0.00046649354,0.00029289996,0.0002688917,0.0009901881],"category_scores_gemma":[0.0005003883,0.00013647237,0.0001447609,0.0009477062,0.00019464437,0.00013797448,0.00044730862,0.0003025009,0.0002619547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040024606,0.00018930489,0.8701713,0.000070825554,0.000055532262,0.0015725336,0.00037619114,0.00073699903,0.10685097,0.0003214769,0.0010916999,0.018162977],"study_design_scores_gemma":[0.000007439777,0.00005667702,0.99667954,0.0000043688,0.000011738831,0.0006911336,0.000057017543,0.00044513788,0.0011304443,0.000034602814,0.0008764286,0.000005385999],"about_ca_topic_score_codex":0.005922787,"about_ca_topic_score_gemma":0.013420052,"teacher_disagreement_score":0.005922787,"about_ca_system_score_codex":0.00043050168,"about_ca_system_score_gemma":0.00022149282,"threshold_uncertainty_score":0.011776626},"labels":[],"label_agreement":null},{"id":"W2047631166","doi":"10.1088/0004-637x/761/2/170","title":"THE SL2S GALAXY-SCALE GRAVITATIONAL LENS SAMPLE. I. THE ALIGNMENT OF MASS AND LIGHT IN MASSIVE EARLY-TYPE GALAXIES AT<i>z</i>= 0.2-0.9","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Gravitational lens; Galaxy; Mass distribution; Dark matter; Astronomy; Weak gravitational lensing; COSMIC cancer database; Gravitation; Telescope; Lens (geology); Redshift; Optics","score_opus":0.008209297236285952,"score_gpt":0.21147255186297687,"score_spread":0.20326325462669093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047631166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99715155,0.000047376816,0.00008503966,0.000016183965,0.0000011839646,0.000007426,0.0022914717,0.000014448258,0.00038530893],"genre_scores_gemma":[0.9903233,0.000043831227,0.00040930655,0.00001965973,0.0000104431865,0.000012784427,0.00853056,0.000008332737,0.00064180745],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998179,0.000025940977,0.000017362301,0.00004758448,0.000048110687,0.000043041666],"domain_scores_gemma":[0.99926525,0.000050507122,0.00026976762,0.00011123872,0.00007615374,0.000227038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036276312,0.0003547271,0.0002711903,0.0016504822,0.0003312098,0.00038076923,0.00028714002,0.00017702662,0.0012948606],"category_scores_gemma":[0.0006876041,0.00015468222,0.0002566159,0.0012523624,0.00021828202,0.00031268052,0.0008534075,0.00013610096,0.000517543],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015259131,0.00003339615,0.9913686,0.000015347168,0.000060804734,0.000120153774,0.00023296237,0.00010868579,0.003249904,0.00010124496,0.000712562,0.0038438172],"study_design_scores_gemma":[0.00001167969,0.000028766046,0.9985708,0.0000017848055,0.000012322995,0.00012021775,0.000104340565,0.00017245905,0.0003091388,0.000023963683,0.0006418707,0.00000253846],"about_ca_topic_score_codex":0.015058631,"about_ca_topic_score_gemma":0.04456839,"teacher_disagreement_score":0.015058631,"about_ca_system_score_codex":0.00039276484,"about_ca_system_score_gemma":0.00023416708,"threshold_uncertainty_score":0.029941976},"labels":[],"label_agreement":null},{"id":"W2047650990","doi":"10.1086/499094","title":"A Burst and Simultaneous Short‐Term Pulsed Flux Enhancement from the Magnetar Candidate 1E 1048.1−5937","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Flux (metallurgy); Astronomy; Neutron star; Chemistry","score_opus":0.006716242267102262,"score_gpt":0.27036264576804087,"score_spread":0.2636464035009386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047650990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991166,0.00009687989,0.00006263961,0.00001863844,0.000005496366,0.000002987881,0.00009247016,0.000008592669,0.0005957025],"genre_scores_gemma":[0.99833125,0.000089028275,0.00034522347,0.000027871845,0.00001873847,0.0000043069267,0.0005396731,0.0000064246506,0.00063762855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999928,0.0000036534873,0.0000041023472,0.000022903412,0.000017869188,0.00002348717],"domain_scores_gemma":[0.9998474,0.00001703787,0.000056840472,0.000017497623,0.000017073491,0.000044165736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000788763,0.00020690978,0.00026942932,0.00042116016,0.0003941125,0.00041008572,0.0002782126,0.00030308406,0.00095215184],"category_scores_gemma":[0.0001951329,0.00011755231,0.0001237089,0.00038327463,0.00018407499,0.00014816079,0.00040805477,0.00028201417,0.0003046435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010994398,0.00024541575,0.5257705,0.000169361,0.00011015025,0.019613618,0.0012745055,0.0005353055,0.41419068,0.0006569617,0.002050411,0.03428357],"study_design_scores_gemma":[0.000019073466,0.00045749175,0.9749978,0.000013063636,0.00004105995,0.009002222,0.00023231319,0.00046085526,0.010704283,0.00011751634,0.0039359783,0.000018376777],"about_ca_topic_score_codex":0.0015656912,"about_ca_topic_score_gemma":0.0032391502,"teacher_disagreement_score":0.0015656912,"about_ca_system_score_codex":0.0002353406,"about_ca_system_score_gemma":0.000117580785,"threshold_uncertainty_score":0.0031852722},"labels":[],"label_agreement":null},{"id":"W2047758030","doi":"10.1088/0004-637x/761/2/139","title":"A POPULATION OF<i>z</i>&gt; 2 FAR-INFRARED<i>HERSCHEL</i>-SPIRE-SELECTED STARBURSTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of British Columbia","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Centre National d’Etudes Spatiales; Key Programme; Science and Technology Facilities Council; Centre National de la Recherche Scientifique; National Science Foundation; Imperial College London; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Space Telescope Science Institute; UK Space Agency","keywords":"Physics; Astrophysics; Spire (mollusc); Redshift; Galaxy; Star formation; Astronomy; Luminous infrared galaxy; Infrared; Population; Far infrared","score_opus":0.007572323283912259,"score_gpt":0.21358462058402025,"score_spread":0.206012297300108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047758030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99743503,0.00009740654,0.00023192646,0.00003186291,0.0000019095532,0.000015885613,0.0007746824,0.000027586124,0.001383658],"genre_scores_gemma":[0.99690706,0.000064332686,0.0003033364,0.000052483676,0.0000071091276,0.000012836483,0.0018808116,0.0000075877024,0.0007644371],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967456,0.000024031937,0.000017954704,0.00013313409,0.000053593132,0.0000966826],"domain_scores_gemma":[0.9994437,0.000052035517,0.00020371971,0.00006915711,0.00006446858,0.0001669143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037064106,0.00019218883,0.000265753,0.0010660772,0.00049069413,0.0006453395,0.000408582,0.00018884751,0.0024060202],"category_scores_gemma":[0.00058505544,0.00012233383,0.0001460481,0.00080877345,0.00042595807,0.0005144113,0.0006557154,0.00018150479,0.00072894007],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011056043,0.00005347031,0.98326254,0.000018106559,0.000028652303,0.00012430751,0.00062002195,0.00012165533,0.0055556977,0.00033612887,0.00057741906,0.009191395],"study_design_scores_gemma":[0.0000054545253,0.000050416893,0.9980311,0.0000026407522,0.000008862413,0.00031888412,0.00018895352,0.00015421376,0.00037908735,0.00007750607,0.0007796377,0.0000032552136],"about_ca_topic_score_codex":0.0058277617,"about_ca_topic_score_gemma":0.007964405,"teacher_disagreement_score":0.0058277617,"about_ca_system_score_codex":0.00029568464,"about_ca_system_score_gemma":0.0001435677,"threshold_uncertainty_score":0.011587679},"labels":[],"label_agreement":null},{"id":"W2047781773","doi":"10.1088/0004-637x/691/2/1248","title":"MERGER-INDUCED GLOBULAR CLUSTER FORMATION AND GALAXY EVOLUTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Dwarf galaxy; Galaxy cluster; Dwarf spheroidal galaxy; Galaxy formation and evolution; Astronomy; Metallicity; Elliptical galaxy; Brightest cluster galaxy; Galaxy; Interacting galaxy","score_opus":0.009233527153527077,"score_gpt":0.2194085638350786,"score_spread":0.21017503668155152,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047781773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9877115,0.00060165854,0.005807976,0.00030432295,0.000013784781,0.00002035004,0.00011204303,0.00004193279,0.005386443],"genre_scores_gemma":[0.9985934,0.00016321756,0.0005203038,0.00002758197,0.0000058850765,0.0000047864223,0.000049285853,0.0000035649375,0.00063202385],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986565,0.00003928553,0.0000049492655,0.000034724813,0.000018736457,0.000036579855],"domain_scores_gemma":[0.99974114,0.000064919215,0.000103155675,0.000022033266,0.000021414924,0.00004728814],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026371813,0.0002343212,0.00023090882,0.000287594,0.00034616748,0.0009990523,0.00056370837,0.00072849286,0.0010713174],"category_scores_gemma":[0.0012540234,0.00015731501,0.00028167185,0.0003142099,0.00071218435,0.00067448517,0.0005989002,0.000274087,0.00017078336],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030402179,0.00019440423,0.2793131,0.00015075688,0.00017177722,0.0011420439,0.0010196321,0.4743922,0.018860787,0.20818232,0.0017886997,0.014480225],"study_design_scores_gemma":[0.0001370977,0.00031244638,0.18082425,0.00003660615,0.00014530092,0.00076435466,0.00036304313,0.7487581,0.0031301258,0.059758406,0.0057000895,0.00007012917],"about_ca_topic_score_codex":0.01362679,"about_ca_topic_score_gemma":0.009467161,"teacher_disagreement_score":0.01362679,"about_ca_system_score_codex":0.0023381528,"about_ca_system_score_gemma":0.0004501716,"threshold_uncertainty_score":0.02709496},"labels":[],"label_agreement":null},{"id":"W2047786967","doi":"10.1088/0004-637x/730/2/131","title":"THE X-RAY POLARIZATION SIGNATURE OF QUIESCENT MAGNETARS: EFFECT OF MAGNETOSPHERIC SCATTERING AND VACUUM POLARIZATION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Magnetosphere; Photon; Polarization (electrochemistry); Soft photon; Magnetar; Astrophysics; Computational physics; Pulsar; Bremsstrahlung; Plasma; Optics; Quantum mechanics","score_opus":0.006178346559885247,"score_gpt":0.2474626575024366,"score_spread":0.24128431094255134,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047786967","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969428,0.000098533164,0.0021006148,0.00003069714,0.0000027903445,0.000003759513,0.000041705975,0.000044577486,0.0007345451],"genre_scores_gemma":[0.9996307,0.000028361785,0.0002469899,0.00000482669,0.0000016635477,0.0000013367465,0.000027268734,0.000009221133,0.00004966221],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992466,0.00002349753,0.000003752398,0.000014930257,0.00001158581,0.000021701882],"domain_scores_gemma":[0.99957615,0.00023415478,0.00007055938,0.00004415851,0.00003167569,0.000043351763],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030310688,0.00034887172,0.00019421629,0.0002766755,0.00024621125,0.0005258655,0.0002468221,0.00023512261,0.00046115307],"category_scores_gemma":[0.0010957707,0.00017549506,0.00032232708,0.00027865192,0.00043416358,0.0003272459,0.00031704083,0.00017649826,0.00007530499],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015202619,0.00017146321,0.38750675,0.00012991905,0.00019268386,0.0009879583,0.0003952796,0.37958544,0.2072081,0.0046575987,0.0003332817,0.017311236],"study_design_scores_gemma":[0.00007440022,0.0002863811,0.17844433,0.000015932474,0.00008296905,0.00030254538,0.000144452,0.76888555,0.04964075,0.0016589073,0.0004246794,0.00003914403],"about_ca_topic_score_codex":0.0020465457,"about_ca_topic_score_gemma":0.0011427776,"teacher_disagreement_score":0.0020465457,"about_ca_system_score_codex":0.00024450797,"about_ca_system_score_gemma":0.00015022524,"threshold_uncertainty_score":0.004069209},"labels":[],"label_agreement":null},{"id":"W2047884563","doi":"10.1088/0004-637x/764/2/133","title":"A FIRST LOOK AT THE AURIGA-CALIFORNIA GIANT MOLECULAR CLOUD WITH<i>HERSCHEL</i>AND THE CSO: CENSUS OF THE YOUNG STELLAR OBJECTS AND THE DENSE GAS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Stars; Young stellar object; Star formation; Spire (mollusc); Astronomy","score_opus":0.0037890567214850816,"score_gpt":0.18058281639942833,"score_spread":0.17679375967794325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047884563","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9434696,0.0032230606,0.00060166913,0.00071483373,0.000039346385,0.000075528886,0.028850278,0.0001330505,0.02289263],"genre_scores_gemma":[0.94927454,0.0032279298,0.005375239,0.0003419771,0.000099234836,0.000046896097,0.03154695,0.00006647346,0.010020739],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999217,0.0000036737074,0.0000053718786,0.000024315246,0.000025784379,0.000019185478],"domain_scores_gemma":[0.9996351,0.000027274653,0.0000961213,0.000032617343,0.000096854674,0.00011192358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011499213,0.00013155535,0.00013162161,0.0020146873,0.0006568991,0.0006184764,0.0002607099,0.00022419674,0.0042134067],"category_scores_gemma":[0.00028441785,0.000107221895,0.00013535496,0.0022575336,0.00016639904,0.00050238747,0.00045716143,0.0003071302,0.00048536793],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007322851,0.000053175034,0.9418067,0.00013168079,0.000045021985,0.00026863007,0.0008090606,0.00033651854,0.00730902,0.0006647412,0.01141662,0.037085626],"study_design_scores_gemma":[0.0000018412856,0.000008641103,0.9857997,0.00001739593,0.0000046966843,0.00007095357,0.0002062866,0.000059106213,0.0002112442,0.000028284707,0.013588694,0.000003240015],"about_ca_topic_score_codex":0.13741349,"about_ca_topic_score_gemma":0.37293875,"teacher_disagreement_score":0.13741349,"about_ca_system_score_codex":0.0006122668,"about_ca_system_score_gemma":0.0005923341,"threshold_uncertainty_score":0.27322733},"labels":[],"label_agreement":null},{"id":"W2047885655","doi":"10.1088/0004-637x/709/2/632","title":"MODELING THE RADIO EMISSION FROM Cyg OB2 NO. 5: A QUADRUPLE SYSTEM?","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Calgary; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Primary (astronomy); Binary number; Astronomy; Supergiant; Binary system; Stars","score_opus":0.009765763283059016,"score_gpt":0.2162068075139399,"score_spread":0.2064410442308809,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047885655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9918937,0.00015953094,0.0062057823,0.00009816202,0.000007822834,0.00001832552,0.00016582853,0.00005646876,0.0013943609],"genre_scores_gemma":[0.9978708,0.000051802526,0.0013368943,0.0000162243,0.0000053020444,0.00001220633,0.00013878738,0.000013974356,0.000553959],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999045,0.000013921533,0.000003591715,0.000039209208,0.000011270668,0.000027450391],"domain_scores_gemma":[0.9998418,0.00004168982,0.000055403856,0.000015727337,0.00001478322,0.00003059942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022240703,0.00034553095,0.00029810137,0.00034259396,0.00030939197,0.000618159,0.00071437546,0.00087125524,0.00105288],"category_scores_gemma":[0.00055312354,0.0002690494,0.00043446504,0.00028167988,0.00031051517,0.0005380461,0.00040535946,0.00034997636,0.000285711],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020863574,0.00015692147,0.17419818,0.00013054548,0.00014003708,0.0006995821,0.00029593057,0.79263407,0.0147091225,0.0034437324,0.0007196804,0.012663584],"study_design_scores_gemma":[0.00001759231,0.00005746608,0.03469569,0.00000785715,0.000033398606,0.0001987916,0.00006162647,0.96237046,0.000954045,0.00079955405,0.00078679033,0.000016663533],"about_ca_topic_score_codex":0.014003706,"about_ca_topic_score_gemma":0.011379124,"teacher_disagreement_score":0.014003706,"about_ca_system_score_codex":0.0007725154,"about_ca_system_score_gemma":0.0003690573,"threshold_uncertainty_score":0.02784437},"labels":[],"label_agreement":null},{"id":"W2047896579","doi":"10.1088/0004-637x/759/1/29","title":"A<i>HST</i>/WFC3-IR MORPHOLOGICAL SURVEY OF GALAXIES AT<i>z</i>= 1.5-3.6. II. THE RELATION BETWEEN MORPHOLOGY AND GAS-PHASE KINEMATICS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"California Institute of Technology; W. M. Keck Foundation; National Aeronautics and Space Administration","keywords":"Galaxy; Redshift; Tully–Fisher relation; Disc galaxy; Outflow; Spectral line; Interstellar medium; Line (geometry); Kinematics; Equivalent width","score_opus":0.022652635395249917,"score_gpt":0.25439857398222726,"score_spread":0.23174593858697734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047896579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9302549,0.0002063941,0.00030175713,0.00007261736,0.000005809303,0.00006278986,0.06569658,0.00019499747,0.0032042149],"genre_scores_gemma":[0.8421341,0.00030490095,0.0025721875,0.00011076611,0.000030283678,0.00012337636,0.15136805,0.00007083976,0.0032855195],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997782,0.000017320086,0.000027790224,0.000052040323,0.000048170023,0.00007651067],"domain_scores_gemma":[0.99864787,0.0000663389,0.0006955391,0.00012978385,0.00016759343,0.00029278276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028055423,0.00033460095,0.0003453286,0.0066619227,0.0003307964,0.0004801354,0.00043520326,0.00029389298,0.00404683],"category_scores_gemma":[0.00052284467,0.00017955451,0.00032441606,0.0052838568,0.00025585294,0.00044885892,0.00053857383,0.00025344835,0.0024609282],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011736168,0.00008751349,0.9763507,0.00007559099,0.0000886233,0.00011411995,0.00027714134,0.00011461665,0.0070059216,0.0001647099,0.0061977278,0.0094059175],"study_design_scores_gemma":[0.0000020648788,0.000011848,0.9986695,0.000002671902,0.000006124952,0.000054607714,0.000043502245,0.00004520693,0.00018220634,0.0000075133134,0.0009732534,0.0000015919363],"about_ca_topic_score_codex":0.023109153,"about_ca_topic_score_gemma":0.034215398,"teacher_disagreement_score":0.023109153,"about_ca_system_score_codex":0.00044131392,"about_ca_system_score_gemma":0.0003467321,"threshold_uncertainty_score":0.04594928},"labels":[],"label_agreement":null},{"id":"W2047953726","doi":"10.1086/522575","title":"Infrared Emission from the Nearby Cool Core Cluster Abell 2597","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Spitzer Space Telescope; Astronomy; Galaxy; Type-cD galaxy; Spectral energy distribution; Galaxy cluster; Luminous infrared galaxy; Luminosity; Photometry (optics); Star formation; Stars","score_opus":0.009486462816052121,"score_gpt":0.22425437813778004,"score_spread":0.21476791532172793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047953726","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925954,0.00012562904,0.000065021835,0.00017067228,0.000057999252,0.000007589685,0.0008263064,0.00007118996,0.0060801827],"genre_scores_gemma":[0.98033005,0.00010975478,0.0002462627,0.00018288547,0.00010221873,0.000008750543,0.003420655,0.00007108902,0.015528188],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99988794,0.0000042291886,0.0000029840971,0.000028385644,0.00004280402,0.000033601744],"domain_scores_gemma":[0.9996191,0.00003216043,0.000049681294,0.000025764386,0.0000904776,0.0001828111],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013139087,0.00016767209,0.00029735512,0.00048703983,0.00083869917,0.00044007672,0.00026325465,0.00036621737,0.009294101],"category_scores_gemma":[0.00030001882,0.00016649823,0.00009507097,0.0003276352,0.00015309396,0.00016195945,0.00040648822,0.00023424746,0.002041417],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0027240792,0.00036225663,0.25335243,0.00029657275,0.00009141223,0.0025388522,0.0008259982,0.00036953733,0.6773192,0.00079282775,0.03405808,0.027268732],"study_design_scores_gemma":[0.000043674063,0.00010239682,0.98700863,0.000009413794,0.000024957671,0.00018702337,0.0001522965,0.00024072932,0.006515555,0.00008540885,0.0056178574,0.000012107844],"about_ca_topic_score_codex":0.006704086,"about_ca_topic_score_gemma":0.016661312,"teacher_disagreement_score":0.009294101,"about_ca_system_score_codex":0.00035766148,"about_ca_system_score_gemma":0.00021012897,"threshold_uncertainty_score":0.03109181},"labels":[],"label_agreement":null},{"id":"W2047985534","doi":"10.1086/504254","title":"The Expansion Asymmetry and Age of the Cassiopeia A Supernova Remnant","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":316,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Ejecta; Cassiopeia A; Supernova remnant; Physics; Asymmetry; Astrophysics; Supernova; Knot (papermaking); Geology; Astronomy","score_opus":0.007627811094828423,"score_gpt":0.21506965098540703,"score_spread":0.2074418398905786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047985534","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99511695,0.0002600589,0.00029733017,0.000023775106,0.000005112717,0.000005801971,0.0011256122,0.000026996357,0.003138431],"genre_scores_gemma":[0.99784684,0.00016964847,0.00022164981,0.000007139478,0.000008247196,0.000004237797,0.0013750055,0.000009547446,0.00035773302],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999107,0.000006093539,0.00000823125,0.00003917185,0.000020267198,0.000015524869],"domain_scores_gemma":[0.99926144,0.000115125426,0.00030053253,0.00007700117,0.000120537596,0.00012529288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033808273,0.00015557253,0.000115569135,0.0012867956,0.00025739658,0.00058364467,0.00014370398,0.00014303914,0.0010844629],"category_scores_gemma":[0.00089856377,0.00013665741,0.00013661428,0.0005422155,0.00022461287,0.0002834382,0.0003182206,0.00021096933,0.0003775888],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029469773,0.000019651865,0.9481772,0.000022249884,0.000046201465,0.00038771954,0.00015195526,0.0010231693,0.041026697,0.0004372724,0.00046651126,0.0079467455],"study_design_scores_gemma":[0.0000016228828,0.000012147606,0.99879825,0.0000026620314,0.000004115759,0.00014079025,0.000015740317,0.00019610199,0.00044683286,0.000031934676,0.00034725285,0.0000025650972],"about_ca_topic_score_codex":0.008640322,"about_ca_topic_score_gemma":0.008691579,"teacher_disagreement_score":0.008640322,"about_ca_system_score_codex":0.00040924118,"about_ca_system_score_gemma":0.0001865839,"threshold_uncertainty_score":0.017180026},"labels":[],"label_agreement":null},{"id":"W2047988398","doi":"10.1086/591654","title":"<i>Chandra</i>Confirmation of a Pulsar Wind Nebula in DA 495","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics; University of Manitoba","funders":"","keywords":"Physics; Pulsar; Nebula; Astrophysics; Pulsar wind nebula; Vela; Neutron star; Astronomy; Luminosity; Supernova remnant; Emission nebula; Supernova; Stars; Galaxy","score_opus":0.017648721012890986,"score_gpt":0.30209529280757824,"score_spread":0.28444657179468724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2047988398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.992235,0.00041658952,0.00044093604,0.00010912731,0.000030509675,0.000017390768,0.00063795387,0.00003562744,0.0060767643],"genre_scores_gemma":[0.99763167,0.000111107816,0.0007707577,0.00007054129,0.000028746064,0.00000568581,0.0007277188,0.0000057972447,0.0006478851],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999422,0.000004423575,0.0000069718285,0.000015172337,0.000016400298,0.000014833158],"domain_scores_gemma":[0.9997925,0.000016732922,0.00006323291,0.000025428182,0.000029966692,0.00007215319],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012210564,0.0001914187,0.00015513938,0.0007961596,0.0008082457,0.0005212965,0.00031847373,0.00026698445,0.0022854612],"category_scores_gemma":[0.00024929835,0.000102063954,0.00015700272,0.00037649338,0.00022878965,0.00020615006,0.0005884579,0.0002569109,0.00054131873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010096201,0.00019153288,0.4995091,0.0002201813,0.00014978448,0.024454666,0.0011053536,0.00032977483,0.44300774,0.0026567488,0.0026308584,0.024734607],"study_design_scores_gemma":[0.00002258024,0.0002305624,0.9678861,0.000023170805,0.000039398066,0.011519443,0.00034310643,0.00036708458,0.009485057,0.00025579898,0.009812728,0.000014925111],"about_ca_topic_score_codex":0.004411443,"about_ca_topic_score_gemma":0.010192662,"teacher_disagreement_score":0.004411443,"about_ca_system_score_codex":0.00026336685,"about_ca_system_score_gemma":0.00016193614,"threshold_uncertainty_score":0.008771479},"labels":[],"label_agreement":null},{"id":"W2048109974","doi":"10.1088/0004-637x/698/2/1872","title":"DEEP 2MASS PHOTOMETRY OF M67 AND CALIBRATION OF THE MAIN-SEQUENCE<i>J</i>–<i>K<sub>S</sub></i>COLOR DIFFERENCE AS AN AGE INDICATOR","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Photometry (optics); Physics; Open cluster; Astrophysics; Stars; Sky; Proper motion; Astronomy; Main sequence; Red clump; Horizontal branch; Milky Way; Globular cluster","score_opus":0.009988220466611205,"score_gpt":0.22594548038586926,"score_spread":0.21595725991925804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048109974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99607,0.000117293086,0.0014931689,0.00002593489,0.0000049388823,0.000008341732,0.00065325695,0.000028015065,0.0015989357],"genre_scores_gemma":[0.9952931,0.00014336429,0.0018754259,0.000022459955,0.000009230266,0.000008185295,0.0018558158,0.000013752283,0.00077853573],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992514,0.000007373993,0.0000037705977,0.000016476315,0.000029028239,0.000018152836],"domain_scores_gemma":[0.9997336,0.000027648985,0.00011047198,0.000038282767,0.00005311965,0.000036755904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016781733,0.00025231877,0.00012336129,0.0009584027,0.00020582697,0.00025134633,0.000154461,0.00014692654,0.0011113802],"category_scores_gemma":[0.0004266213,0.000116668765,0.00016694207,0.0008073401,0.00013709084,0.00015730961,0.0003252184,0.00013018592,0.0005897021],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007684342,0.000031745585,0.9574864,0.000035432433,0.000022406772,0.00016383431,0.00020220941,0.0021394468,0.020090964,0.0006018919,0.0007437525,0.018405031],"study_design_scores_gemma":[0.0000022305398,0.000036360758,0.9948442,0.000007085154,0.00001027971,0.00012024958,0.00007606493,0.0018829053,0.001427758,0.00010887643,0.0014802238,0.000003938322],"about_ca_topic_score_codex":0.0081592575,"about_ca_topic_score_gemma":0.02867915,"teacher_disagreement_score":0.0081592575,"about_ca_system_score_codex":0.0003128263,"about_ca_system_score_gemma":0.0001569032,"threshold_uncertainty_score":0.01622349},"labels":[],"label_agreement":null},{"id":"W2048116343","doi":"10.1086/518432","title":"Accurate Realizations of the Ionized Gas in Galaxy Clusters: Calibrating Feedback","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Hydrostatic equilibrium; Halo; Galaxy; Galaxy cluster; Cluster (spacecraft); Redshift; Stars; Star cluster","score_opus":0.01017553750883617,"score_gpt":0.2321753442657693,"score_spread":0.22199980675693312,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048116343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942532,0.000031684212,0.004616784,0.000054434608,0.0000058032356,0.000012216249,0.00015164683,0.00013283212,0.000741364],"genre_scores_gemma":[0.9985287,0.000011817285,0.001291143,0.0000055336345,0.0000019967094,0.000008128899,0.00008900615,0.000010958028,0.00005261675],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99978656,0.00006382287,0.000010963526,0.000052919895,0.000041411688,0.00004440377],"domain_scores_gemma":[0.99822205,0.0009147986,0.00019333273,0.00025453686,0.00023459077,0.00018067363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008229072,0.000360902,0.00041217348,0.0004019021,0.00052065053,0.00077797886,0.0011646032,0.00085072656,0.000737476],"category_scores_gemma":[0.0055808383,0.00061712303,0.00034415087,0.00053530355,0.0008535742,0.0007205887,0.0006898923,0.00058758724,0.00010615268],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059612732,0.000021835387,0.010666453,0.0000068460326,0.000017082071,0.0000337834,0.0000459289,0.98672676,0.0004559015,0.0009039876,0.00006988403,0.0009919521],"study_design_scores_gemma":[0.000024504268,0.000020615937,0.0029520716,0.0000023778941,0.0000063745442,0.0000072356947,0.00001537415,0.99562633,0.0003891556,0.0008873361,0.00006168073,0.0000068696886],"about_ca_topic_score_codex":0.029079733,"about_ca_topic_score_gemma":0.014781039,"teacher_disagreement_score":0.029079733,"about_ca_system_score_codex":0.0020440922,"about_ca_system_score_gemma":0.0008976058,"threshold_uncertainty_score":0.057820916},"labels":[],"label_agreement":null},{"id":"W2048195651","doi":"10.1086/503792","title":"Six Peaks Visible in the Redshift Distribution of 46,400 SDSS Quasars Agree with the Preferred Redshifts Predicted by the Decreasing Intrinsic Redshift Model","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Redshift; Quasar; Red shift; Distribution (mathematics); Spectral line; Cosmology; Redshift survey","score_opus":0.007468386827243652,"score_gpt":0.20739938767921645,"score_spread":0.1999310008519728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048195651","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9816799,0.0005025517,0.003902535,0.00037653887,0.00009036088,0.000036373698,0.0031998784,0.0005803187,0.009631557],"genre_scores_gemma":[0.9953551,0.000095451964,0.0010404624,0.00003231438,0.000029141705,0.000005049654,0.0013521176,0.000047623802,0.0020426582],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999466,0.000029653507,0.000038750557,0.000112626374,0.0002019949,0.00015104529],"domain_scores_gemma":[0.9961145,0.0010274904,0.0009028392,0.0005880144,0.0007009542,0.0006662447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008521999,0.00029095422,0.00041517286,0.0013415081,0.0007340673,0.0010854355,0.0005126389,0.0005740246,0.0097676655],"category_scores_gemma":[0.0032570006,0.00031226312,0.0003839713,0.0013386842,0.0004321247,0.00058600947,0.0007658471,0.00050128874,0.0029375944],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008815205,0.00021003405,0.8480036,0.0002927419,0.00010626642,0.0005861215,0.0009446008,0.0014524062,0.049802657,0.005358216,0.008245975,0.084115885],"study_design_scores_gemma":[0.000028053757,0.0000446893,0.9858279,0.000008085294,0.000028985576,0.00024753992,0.00016891545,0.000972727,0.006511072,0.001350179,0.004791893,0.000020033576],"about_ca_topic_score_codex":0.0014373686,"about_ca_topic_score_gemma":0.001877804,"teacher_disagreement_score":0.0097676655,"about_ca_system_score_codex":0.00025563617,"about_ca_system_score_gemma":0.00031440888,"threshold_uncertainty_score":0.03267604},"labels":[],"label_agreement":null},{"id":"W2048241694","doi":"10.1086/508343","title":"Proto-Brown Dwarf Disks as Products of Protostellar Disk Encounters","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Brown dwarf; Physics; Astrophysics; Fragmentation (computing); Stars; Astronomy; Jupiter (rocket family); Computer science; Spacecraft","score_opus":0.007329050632308978,"score_gpt":0.2298829156464046,"score_spread":0.2225538650140956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048241694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99356776,0.00015894086,0.0027702642,0.000050232706,0.00001287111,0.000025609173,0.00011077791,0.00007404841,0.0032295831],"genre_scores_gemma":[0.9974502,0.000085648535,0.0013505411,0.000012032857,0.000004408773,0.000011991376,0.000075735734,0.00001792752,0.0009915527],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984336,0.000043117783,0.0000099879535,0.000024309167,0.00004253006,0.000036619353],"domain_scores_gemma":[0.9993051,0.0002546731,0.00012753275,0.00007415574,0.000066958106,0.0001715195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045014624,0.00036698626,0.0003707026,0.00040139072,0.00059077266,0.0014287701,0.00060904335,0.00061308756,0.0019464708],"category_scores_gemma":[0.0019084603,0.00039136087,0.0004002593,0.00037811612,0.0007244767,0.00084388576,0.0008746306,0.00038482618,0.00026770963],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007042036,0.0002407081,0.11373598,0.00020707615,0.00012020339,0.0027176926,0.0017136508,0.8234252,0.017614597,0.027888767,0.0013537953,0.010278139],"study_design_scores_gemma":[0.0001750649,0.00016746823,0.01574634,0.000022533754,0.000046820558,0.00053581473,0.00042734158,0.9663431,0.0055574444,0.008362849,0.002586821,0.000028356264],"about_ca_topic_score_codex":0.0039811186,"about_ca_topic_score_gemma":0.00265637,"teacher_disagreement_score":0.0039811186,"about_ca_system_score_codex":0.0008370047,"about_ca_system_score_gemma":0.00039033676,"threshold_uncertainty_score":0.007915854},"labels":[],"label_agreement":null},{"id":"W2048316219","doi":"10.1086/590483","title":"AGN Dusty Tori. II. Observational Implications of Clumpiness","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":814,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Seneca Polytechnic","funders":"","keywords":"Physics; Astrophysics; Torus; QSOS; Active galactic nucleus; Astronomy; Circumstellar dust; Galaxy; Cosmic dust; Quasar; Geometry","score_opus":0.04142635428573669,"score_gpt":0.27000772404546713,"score_spread":0.22858136975973045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048316219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99061745,0.00041832778,0.002626625,0.0003940559,0.000016833064,0.000023520517,0.0007753418,0.000096476884,0.0050314246],"genre_scores_gemma":[0.999521,0.000035282268,0.00015610857,0.00001958448,0.00001471665,0.0000034997036,0.0001549463,0.000004684568,0.00009007813],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997173,0.00005162875,0.00001898555,0.00009259805,0.00005472327,0.000064817265],"domain_scores_gemma":[0.99506,0.0014896042,0.0020147674,0.0006816563,0.00027408116,0.00047982493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096668204,0.0002765874,0.00025275772,0.0007779607,0.00051251915,0.00085658603,0.000765017,0.00053799304,0.0018021684],"category_scores_gemma":[0.0057392465,0.0002957467,0.00040922497,0.000494075,0.00071288034,0.0011219997,0.0006890292,0.0006183028,0.0002559642],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000488377,0.000064108266,0.94896096,0.000103893086,0.00008275893,0.0011699928,0.0005403992,0.018308789,0.008848815,0.008894709,0.0017262786,0.0108109275],"study_design_scores_gemma":[0.00009217246,0.00010830471,0.9159362,0.000033889923,0.000050314997,0.0012363968,0.00053550105,0.062612616,0.0018782989,0.015114538,0.0023757787,0.000026082871],"about_ca_topic_score_codex":0.007207836,"about_ca_topic_score_gemma":0.004608266,"teacher_disagreement_score":0.007207836,"about_ca_system_score_codex":0.0010244879,"about_ca_system_score_gemma":0.00014871733,"threshold_uncertainty_score":0.014331758},"labels":[],"label_agreement":null},{"id":"W2048401875","doi":"10.1086/308427","title":"Doppler Imaging of VW Cephei: Distribution and Evolution of Starspots on a Contact Binary","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Starspot; Physics; Astrophysics; Spots; Polar; Light curve; Differential rotation; Contact binary; Doppler effect; Asymmetry; Binary star; Cold spot; Astronomy; Stars","score_opus":0.006025196848042381,"score_gpt":0.21070282684207528,"score_spread":0.2046776299940329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048401875","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989801,0.00006593233,0.00017190039,0.000008897792,0.0000011821426,0.000002689468,0.00024921884,0.0000136339995,0.0005064615],"genre_scores_gemma":[0.9993111,0.000017187265,0.0002524516,0.000001567539,0.000003933096,0.0000018132304,0.00035543542,0.0000026630378,0.000053866843],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988806,0.000011127986,0.000004682723,0.000028195334,0.00003389906,0.000034086726],"domain_scores_gemma":[0.99942243,0.0001418926,0.00018068882,0.000048714595,0.00008830525,0.00011795191],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001815825,0.00015382003,0.0002470498,0.0020484263,0.0003322398,0.00044089323,0.00022203286,0.0002621006,0.0006277448],"category_scores_gemma":[0.0009245608,0.00015626744,0.0001352872,0.0011069397,0.00018928431,0.00026885245,0.0003652669,0.00017552184,0.00013013925],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049250777,0.000106386506,0.9126194,0.00006472106,0.000057621444,0.0007444349,0.00076036557,0.003107421,0.053942963,0.00055501534,0.0007831794,0.026765946],"study_design_scores_gemma":[0.000003786693,0.00002426734,0.99453706,0.000003841167,0.000008369949,0.0002163143,0.00006252685,0.0031481504,0.0015996243,0.00006651132,0.00032469002,0.000004860806],"about_ca_topic_score_codex":0.0027659538,"about_ca_topic_score_gemma":0.0048572444,"teacher_disagreement_score":0.0027659538,"about_ca_system_score_codex":0.00041118963,"about_ca_system_score_gemma":0.00009192523,"threshold_uncertainty_score":0.0054997206},"labels":[],"label_agreement":null},{"id":"W2048414192","doi":"10.1088/0004-637x/798/2/123","title":"OGLE-2013-BLG-0102LA,B: MICROLENSING BINARY WITH COMPONENTS AT STAR/BROWN DWARF AND BROWN DWARF/PLANET BOUNDARIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Gravitational microlensing; Gravitational lens; Light curve; Caustic (mathematics); Lens (geology); Binary number; Anomaly (physics); Proper motion","score_opus":0.020337963442689046,"score_gpt":0.27635424899375416,"score_spread":0.2560162855510651,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048414192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99580705,0.00009443561,0.0004463484,0.00003677598,0.000008032569,0.000022477896,0.001524115,0.00009702745,0.00196367],"genre_scores_gemma":[0.99536926,0.000022741166,0.0006552592,0.000022039287,0.0000101547685,0.000008835818,0.0034895919,0.000016722115,0.00040536124],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981266,0.00001075282,0.000009439057,0.000044134897,0.00004017785,0.000082853614],"domain_scores_gemma":[0.9994886,0.000052159583,0.00019149271,0.00003839494,0.000038329123,0.00019096347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019223172,0.00039077108,0.00042697543,0.001512875,0.00070663827,0.00088904804,0.00029099,0.0005745137,0.0016575877],"category_scores_gemma":[0.00044340861,0.00014883706,0.00041874457,0.0012709511,0.00028048496,0.0002234134,0.00077876437,0.00031600008,0.0004089598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022279175,0.00047129788,0.9112641,0.00015959828,0.00022437613,0.008736975,0.00038791573,0.0050939773,0.0424536,0.0027728865,0.0039519602,0.022255335],"study_design_scores_gemma":[0.00005013263,0.00007991088,0.9854569,0.000007782719,0.000031265987,0.0019454852,0.00014549473,0.006545456,0.0032998878,0.00025167014,0.0021683997,0.00001755034],"about_ca_topic_score_codex":0.011877697,"about_ca_topic_score_gemma":0.015777584,"teacher_disagreement_score":0.011877697,"about_ca_system_score_codex":0.000982489,"about_ca_system_score_gemma":0.0003951389,"threshold_uncertainty_score":0.023617089},"labels":[],"label_agreement":null},{"id":"W2048501582","doi":"10.1088/0004-637x/693/1/552","title":"PREDICTIONS OF QUASAR CLUSTERING: REDSHIFT, LUMINOSITY, AND SELECTION DEPENDENCE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Redshift; Quasar; Luminosity; Sky; Correlation function (quantum field theory); Cluster analysis; Halo; Amplitude; Correlation; Range (aeronautics); Luminosity function; Galaxy; Optics; Statistics","score_opus":0.008408343847694011,"score_gpt":0.22017053337002698,"score_spread":0.21176218952233297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048501582","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9492333,0.00021872112,0.043777637,0.00041418077,0.000014964063,0.000021334323,0.0004253123,0.00034220284,0.005552387],"genre_scores_gemma":[0.99669576,0.00008888879,0.00235765,0.00005894996,0.000011417079,0.000014410589,0.00017375802,0.00004367378,0.0005555271],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981004,0.000049571267,0.000006933698,0.000050393788,0.0000373222,0.000045804103],"domain_scores_gemma":[0.99802303,0.0009972526,0.0003873155,0.00021909951,0.00020019297,0.00017319575],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096155686,0.00041109516,0.00035273776,0.0006305051,0.00037289818,0.00074417784,0.00096336054,0.0006375594,0.0016247683],"category_scores_gemma":[0.005667922,0.00033553335,0.00047747386,0.00048016972,0.0006490162,0.00085797504,0.00037969448,0.0004197009,0.00052564923],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043436903,0.000034499422,0.06636778,0.000017057764,0.000030052934,0.000066068205,0.000059436014,0.9201015,0.0012061164,0.0077927783,0.0006996208,0.0035816298],"study_design_scores_gemma":[0.000012975939,0.000011262956,0.013217913,0.00000559589,0.000008440795,0.000024405877,0.000012951103,0.9823966,0.00033450327,0.003808785,0.00015544413,0.000011167881],"about_ca_topic_score_codex":0.020459382,"about_ca_topic_score_gemma":0.012882113,"teacher_disagreement_score":0.020459382,"about_ca_system_score_codex":0.001149104,"about_ca_system_score_gemma":0.0005490999,"threshold_uncertainty_score":0.040680587},"labels":[],"label_agreement":null},{"id":"W2048534291","doi":"10.1088/0004-637x/781/2/95","title":"GEMS IN THE OUTER GALAXY: NEAR-INFRARED IMAGING OF THREE YOUNG CLUSTERS AT LARGE GALACTIC RADII","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Galaxy; Solar mass; Stars; Astronomy; Sky; Open cluster; Star cluster; Solar System; Main sequence; Cluster (spacecraft)","score_opus":0.008609211035403826,"score_gpt":0.21630095982526795,"score_spread":0.20769174878986413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048534291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986835,0.0000509244,0.0001958369,0.000011221545,0.00000203419,0.000004037892,0.0002583344,0.000045747565,0.0007483293],"genre_scores_gemma":[0.9969777,0.00005626995,0.0014393292,0.000014888768,0.000005186632,0.000006142519,0.0010033333,0.000017611497,0.0004794196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992096,0.0000046355867,0.000004522925,0.000024091332,0.000023931407,0.00002185481],"domain_scores_gemma":[0.99975556,0.000014986415,0.00005325752,0.000021680009,0.000036182504,0.00011825448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019675438,0.00014518126,0.00016218121,0.0015319218,0.00038716412,0.00026239437,0.00021561178,0.00018682904,0.0007656139],"category_scores_gemma":[0.0001815593,0.00015421728,0.00016265434,0.00066836306,0.0001487094,0.00019994445,0.00061258324,0.0001758029,0.00032478926],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068148517,0.00020547859,0.70529354,0.00007434415,0.00014727261,0.00089605124,0.001799664,0.0014209264,0.2471426,0.0005780767,0.0022907518,0.0394698],"study_design_scores_gemma":[0.0000031786324,0.000023886168,0.9967049,0.0000024131564,0.000009435651,0.00019818569,0.00016655344,0.0006902102,0.0017005949,0.000030594027,0.00046650943,0.000003582326],"about_ca_topic_score_codex":0.005598995,"about_ca_topic_score_gemma":0.01285977,"teacher_disagreement_score":0.005598995,"about_ca_system_score_codex":0.00031562583,"about_ca_system_score_gemma":0.00014092555,"threshold_uncertainty_score":0.011132777},"labels":[],"label_agreement":null},{"id":"W2048536046","doi":"10.1086/522488","title":"Horizontal Branch Evolution and Atomic Diffusion","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Horizontal branch; Physics; Diffusion; Astrophysics; Stars; Red-giant branch; Stellar evolution; Hertzsprung–Russell diagram; Atomic diffusion; Luminosity; Hydrogen; Thermodynamics; Metallicity; Quantum mechanics","score_opus":0.0057162136488802945,"score_gpt":0.21158874236558997,"score_spread":0.2058725287167097,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048536046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78441626,0.010335711,0.01777686,0.015542916,0.0009514314,0.000022211687,0.00076664303,0.00039031162,0.16979758],"genre_scores_gemma":[0.9688237,0.0026386539,0.0017459673,0.00028214612,0.00063544785,0.000006155413,0.00026035038,0.000083286825,0.025524335],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996424,0.000005130659,0.0000013807321,0.0000136969265,0.000008256172,0.0000073162523],"domain_scores_gemma":[0.9991235,0.00039082803,0.0001083866,0.00006760948,0.00015750618,0.00015218576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039001933,0.00014687961,0.00024498143,0.0007589564,0.0006639865,0.0016458045,0.00032695063,0.0007207711,0.015727518],"category_scores_gemma":[0.0025590262,0.0001526555,0.00020532499,0.00097377243,0.0004070767,0.0015873798,0.0006540823,0.00078628113,0.00082471356],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038126082,0.000095322386,0.11008963,0.0002109885,0.0001043821,0.0006562574,0.0012844834,0.033485565,0.02736025,0.605108,0.033240847,0.18798308],"study_design_scores_gemma":[0.00006748865,0.00008402776,0.24037823,0.0001372496,0.00008773894,0.0006582862,0.0010189583,0.09960652,0.0066711223,0.57795024,0.073243245,0.00009685417],"about_ca_topic_score_codex":0.0025275298,"about_ca_topic_score_gemma":0.0018864959,"teacher_disagreement_score":0.015727518,"about_ca_system_score_codex":0.00082226336,"about_ca_system_score_gemma":0.00017356715,"threshold_uncertainty_score":0.052613795},"labels":[],"label_agreement":null},{"id":"W2048665625","doi":"10.1086/512676","title":"Germanium Production in Asymptotic Giant Branch Stars: Implications for Observations of Planetary Nebulae","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Asymptotic giant branch; Nucleosynthesis; Planetary nebula; Astrophysics; Physics; Stars; Abundance (ecology); Germanium; Formation and evolution of the Solar System; Astronomy; Solar System; Silicon","score_opus":0.033128732384985114,"score_gpt":0.2961006335936194,"score_spread":0.2629719012086343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048665625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897656,0.0021431693,0.0039414493,0.00083856547,0.00002903615,0.000010929026,0.00047294825,0.000112821086,0.0026853806],"genre_scores_gemma":[0.9981963,0.00037670432,0.0010334522,0.00003703812,0.000015167717,0.000003850303,0.00016740839,0.00001666153,0.00015353457],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989617,0.000025727742,0.000006938483,0.000033559525,0.000021013175,0.000016626533],"domain_scores_gemma":[0.9995129,0.00028545977,0.00005066226,0.00004801682,0.00005002735,0.000052985597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040408896,0.00044257904,0.00040397377,0.00043316116,0.00035673333,0.00056426285,0.00089184445,0.00081340875,0.0011509478],"category_scores_gemma":[0.0017807379,0.00028928052,0.0006466265,0.0005350408,0.00032898985,0.0006700944,0.00053666625,0.00031269123,0.00014802042],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041303653,0.00011243381,0.7237113,0.00027848317,0.00016280738,0.0011257797,0.00012805212,0.22236308,0.02617681,0.0035713303,0.00079397985,0.021162888],"study_design_scores_gemma":[0.000084514126,0.00012865549,0.57903814,0.00008359812,0.000086706736,0.00054089684,0.000253532,0.4029629,0.0069310605,0.008070804,0.001753621,0.00006553081],"about_ca_topic_score_codex":0.010006581,"about_ca_topic_score_gemma":0.0061719366,"teacher_disagreement_score":0.010006581,"about_ca_system_score_codex":0.0005661837,"about_ca_system_score_gemma":0.00023957218,"threshold_uncertainty_score":0.019896686},"labels":[],"label_agreement":null},{"id":"W2048729458","doi":"10.1088/0004-637x/727/2/80","title":"GRAVITATIONAL LENS MODELING WITH GENETIC ALGORITHMS AND PARTICLE SWARM OPTIMIZERS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Particle swarm optimization; Lens (geology); Algorithm; Nonlinear system; Optimization problem; Mathematical optimization; Regularization (linguistics); Parameter space; Computer science; Mathematics; Physics; Optics; Artificial intelligence; Geometry","score_opus":0.028393599997192043,"score_gpt":0.22569577649889463,"score_spread":0.1973021765017026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048729458","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.008743838,0.00017229104,0.98781556,0.00018955176,0.00002238384,0.000044211043,0.000026857482,0.00021250141,0.0027727215],"genre_scores_gemma":[0.402535,0.0004862244,0.59013236,0.00018677347,0.00007859614,0.0004915914,0.0001409266,0.00016931219,0.005779269],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997341,0.00010996307,0.000012900279,0.000040424657,0.000077300094,0.000025288757],"domain_scores_gemma":[0.9992417,0.00044980497,0.00011930215,0.00004549287,0.00011608606,0.000027503735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00091038254,0.0010650544,0.0007548224,0.00084874814,0.0005075422,0.0010997646,0.0012810724,0.0015101051,0.0010854789],"category_scores_gemma":[0.0024627515,0.0005522762,0.00079686963,0.000753093,0.00092346343,0.00082246005,0.00086456176,0.0009912461,0.00029441825],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000058787086,0.0000060273424,0.00012083541,0.000011034149,0.0000095629475,0.00000979548,0.000014413685,0.9894331,0.00020718499,0.005588527,0.00015219074,0.004441462],"study_design_scores_gemma":[0.0000019423821,0.000002649145,0.000013232228,0.0000017101719,0.0000010436856,0.0000015281158,0.0000020092432,0.99845695,0.000060218466,0.0013388245,0.0001184614,0.0000014892859],"about_ca_topic_score_codex":0.009968486,"about_ca_topic_score_gemma":0.0060270396,"teacher_disagreement_score":0.009968486,"about_ca_system_score_codex":0.0012086619,"about_ca_system_score_gemma":0.0012711146,"threshold_uncertainty_score":0.019820929},"labels":[],"label_agreement":null},{"id":"W2048752668","doi":"10.1088/0004-637x/756/2/119","title":"CONNECTING THE DOTS: ANALYZING SYNTHETIC OBSERVATIONS OF STAR-FORMING CLUMPS IN MOLECULAR CLOUDS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Molecular cloud; Measure (data warehouse); Line (geometry); Star formation; Data cube; Cube (algebra); Column (typography); Projection (relational algebra)","score_opus":0.020258571751982042,"score_gpt":0.25543245865883646,"score_spread":0.23517388690685442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048752668","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963037,0.000039152597,0.003288686,0.000024191686,0.000004477864,0.00001158665,0.0001726512,0.00006469976,0.00009079175],"genre_scores_gemma":[0.995462,0.000016729895,0.0039029343,0.000012956324,0.000004679723,0.000008027643,0.00054493675,0.0000141839155,0.00003357616],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99972945,0.00007392619,0.00001485078,0.00007873786,0.00006128842,0.000041664425],"domain_scores_gemma":[0.997566,0.0012915385,0.00043757752,0.0003291049,0.00020946191,0.00016639936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007856917,0.00034313707,0.00029030695,0.00071430404,0.0002969081,0.0005579375,0.00074644573,0.0005696347,0.00029125842],"category_scores_gemma":[0.0049717617,0.00023921927,0.0004833535,0.00058114453,0.0004730052,0.00054768333,0.0005365576,0.0003441105,0.00006442623],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003560088,0.00021459218,0.21270461,0.000063461455,0.00017067972,0.00038432688,0.00024145683,0.76063836,0.014481951,0.001262104,0.00033807577,0.009144426],"study_design_scores_gemma":[0.000027807073,0.00007476016,0.042095292,0.000004794166,0.0000142203535,0.00007511032,0.00007943709,0.9518627,0.0046421387,0.00089007034,0.00021769365,0.000016011749],"about_ca_topic_score_codex":0.0058293203,"about_ca_topic_score_gemma":0.0047307843,"teacher_disagreement_score":0.0058293203,"about_ca_system_score_codex":0.000558241,"about_ca_system_score_gemma":0.00025481102,"threshold_uncertainty_score":0.011590779},"labels":[],"label_agreement":null},{"id":"W2048873767","doi":"10.1088/0004-637x/777/1/69","title":"A RADIO-SELECTED BLACK HOLE X-RAY BINARY CANDIDATE IN THE MILKY WAY GLOBULAR CLUSTER M62","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Milky Way; Black hole (networking); Jansky; Star cluster; Binary black hole; Intermediate-mass black hole; Stellar black hole","score_opus":0.008220157012006155,"score_gpt":0.2144277035643796,"score_spread":0.20620754655237344,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2048873767","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996259,0.00003629638,0.00003419437,0.000014076232,0.0000016440225,0.0000015231557,0.000013768581,0.0000037593131,0.00026879672],"genre_scores_gemma":[0.999446,0.000021738564,0.00014169837,0.000020263073,0.0000048065076,0.0000012157507,0.000089044595,0.0000017489136,0.0002735666],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993145,0.0000041281614,0.0000046103464,0.00002116147,0.000018509149,0.000020121002],"domain_scores_gemma":[0.9997955,0.000017922745,0.00006111953,0.000022694747,0.000023211058,0.000079507765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011676403,0.00016873398,0.00019854355,0.0004498233,0.0005512197,0.0004176047,0.0002327241,0.00038061116,0.0009981114],"category_scores_gemma":[0.00031869303,0.00011876418,0.00009944209,0.0002662168,0.00024650816,0.00017084574,0.000573357,0.00014460762,0.00030509807],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032341236,0.0000772997,0.9278425,0.000028832712,0.000032653552,0.0055511543,0.0009204528,0.0002431929,0.054663666,0.00045872646,0.00054238166,0.009315742],"study_design_scores_gemma":[0.000028622573,0.00035412886,0.9816467,0.000011770006,0.000032761567,0.0068561453,0.0007048315,0.0011790104,0.0059658065,0.00027258362,0.0029343162,0.00001327863],"about_ca_topic_score_codex":0.0018233663,"about_ca_topic_score_gemma":0.0038152533,"teacher_disagreement_score":0.0018233663,"about_ca_system_score_codex":0.00018010476,"about_ca_system_score_gemma":0.00009917911,"threshold_uncertainty_score":0.0036255121},"labels":[],"label_agreement":null},{"id":"W2049040639","doi":"10.1088/0004-637x/801/1/25","title":"ALMA REVEALS THE MOLECULAR MEDIUM FUELING THE NEAREST NUCLEAR STARBURST","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":212,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Isotopologue; Galaxy; Star formation; Line (geometry); Molecular cloud; Astronomy; Stars; Scaling; Geometry; Spectral line","score_opus":0.017023341369338266,"score_gpt":0.24590735675073605,"score_spread":0.2288840153813978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049040639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99652416,0.00009728864,0.00049728836,0.000021860309,0.0000036344727,0.0000045689826,0.00049142557,0.00007673343,0.0022829561],"genre_scores_gemma":[0.9984541,0.000027076507,0.00076501095,0.000009934355,0.000004993474,0.0000036825327,0.00041030548,0.000004966394,0.00031978264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996316,0.0000017521633,9.888814e-7,0.00001476961,0.0000069938033,0.000012274625],"domain_scores_gemma":[0.99984634,0.00002138738,0.000050038645,0.0000143562875,0.00001837206,0.000049537008],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006181514,0.00010872903,0.00010046442,0.00065724296,0.0002756907,0.00041972895,0.0001971072,0.00019005526,0.0012369439],"category_scores_gemma":[0.00020428687,0.000095161035,0.00012836524,0.00027987402,0.00011514498,0.00022768222,0.00023337694,0.0001897366,0.00024154555],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032956572,0.00009794204,0.7013529,0.00004717847,0.000065086235,0.0008759659,0.0005784938,0.002138999,0.27693063,0.0010227065,0.0010787001,0.015481808],"study_design_scores_gemma":[0.000008031612,0.00005400561,0.98319143,0.000008382355,0.000025027432,0.00023108907,0.0001443685,0.0067749387,0.0067821634,0.00015818502,0.0026149002,0.000007393277],"about_ca_topic_score_codex":0.011511794,"about_ca_topic_score_gemma":0.021915795,"teacher_disagreement_score":0.011511794,"about_ca_system_score_codex":0.00037972615,"about_ca_system_score_gemma":0.000104256476,"threshold_uncertainty_score":0.022889614},"labels":[],"label_agreement":null},{"id":"W2049125838","doi":"10.1088/0004-637x/725/1/750","title":"PARSEC-SCALE FARADAY ROTATION MEASURES FROM GENERAL RELATIVISTIC MAGNETOHYDRODYNAMIC SIMULATIONS OF ACTIVE GALACTIC NUCLEUS JETS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Faraday effect; Active galactic nucleus; Astrophysical jet; Jet (fluid); Magnetohydrodynamics; Astrophysics; Magnetohydrodynamic drive; Computational physics; Galaxy; Magnetic field; Mechanics","score_opus":0.007697455338282888,"score_gpt":0.22327921920478344,"score_spread":0.21558176386650055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049125838","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.979596,0.00024189247,0.009933877,0.00034829855,0.000050552047,0.00004979713,0.00091315125,0.0003606028,0.00850583],"genre_scores_gemma":[0.9943768,0.00012754272,0.0039771744,0.00007322115,0.000026237802,0.00004888491,0.00082890445,0.00010505154,0.00043637498],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986076,0.000042937856,0.000008315101,0.000017508775,0.000033143275,0.000037275648],"domain_scores_gemma":[0.9991634,0.0004604686,0.00012448146,0.00006500439,0.00008602145,0.000100653786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004935121,0.0006659755,0.00038979758,0.00060409756,0.00049315445,0.00087580644,0.0007841808,0.0007683698,0.0013390178],"category_scores_gemma":[0.0028367185,0.00033404698,0.00066741783,0.00054961356,0.0007335977,0.00038659136,0.0006287486,0.00074336707,0.00015645978],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050288258,0.000048612183,0.005101247,0.000020803142,0.000027324331,0.00006623404,0.000049628205,0.9910212,0.00080039556,0.0015470055,0.0003285238,0.0009387131],"study_design_scores_gemma":[0.000028124787,0.000022941413,0.0024476147,0.000005942352,0.0000068683325,0.000012424247,0.00002384997,0.99612683,0.0002671153,0.0008217872,0.00022894127,0.000007579111],"about_ca_topic_score_codex":0.0168426,"about_ca_topic_score_gemma":0.008440182,"teacher_disagreement_score":0.0168426,"about_ca_system_score_codex":0.0009878747,"about_ca_system_score_gemma":0.0006459376,"threshold_uncertainty_score":0.033489108},"labels":[],"label_agreement":null},{"id":"W2049179731","doi":"10.1086/374218","title":"The Initial Helium Content of Galactic Globular Cluster Stars from the<i>R</i>‐Parameter: Comparison with the Cosmic Microwave Background Constraint","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":167,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Cosmic microwave background; Globular cluster; Astrophysics; Physics; Stars; Metallicity; Nucleosynthesis; Big Bang nucleosynthesis; COSMIC cancer database; Astronomy","score_opus":0.03135636455097133,"score_gpt":0.2498898486650196,"score_spread":0.21853348411404827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049179731","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984314,0.00012150078,0.00048918836,0.000010268473,8.2919723e-7,0.0000014561056,0.00023555741,0.00001890328,0.00069098035],"genre_scores_gemma":[0.9989574,0.000038854734,0.0003088992,0.000003287299,0.0000014668099,0.000001120608,0.0005973121,0.0000067556634,0.000084920066],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988616,0.000013125785,0.00000450924,0.000057791858,0.00001700058,0.000021386699],"domain_scores_gemma":[0.9995622,0.00013464346,0.00007265819,0.000076163284,0.00008042705,0.000073803094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034296865,0.00027212946,0.00015664996,0.00091013586,0.00021472799,0.0005407672,0.00041370658,0.0003061298,0.00066474883],"category_scores_gemma":[0.00067265664,0.000104396146,0.00022517618,0.00063989055,0.00025926376,0.00023454113,0.000350663,0.00020255407,0.0002665188],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001057172,0.0000831037,0.9071603,0.000071622446,0.00011949917,0.00019962787,0.00029168904,0.015589973,0.05390103,0.0018174807,0.0005879398,0.01912064],"study_design_scores_gemma":[0.000019633511,0.00006416177,0.9543117,0.0000067815504,0.000044118056,0.00010786637,0.000091254384,0.023387164,0.0204341,0.0004712447,0.0010426837,0.000019283203],"about_ca_topic_score_codex":0.011574962,"about_ca_topic_score_gemma":0.0072670598,"teacher_disagreement_score":0.011574962,"about_ca_system_score_codex":0.0006531818,"about_ca_system_score_gemma":0.00022972717,"threshold_uncertainty_score":0.023015141},"labels":[],"label_agreement":null},{"id":"W2049182449","doi":"10.1086/423267","title":"Models of the Intracluster Medium with Heating and Cooling: Explaining the Global and Structural X‐Ray Properties of Clusters","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; University of Victoria","funders":"","keywords":"Radiative cooling; Intracluster medium; Cooling flow; Surface brightness; Physics; Astrophysics; Radiative transfer; Cluster (spacecraft); Galaxy cluster; Thermal; Entropy (arrow of time); Galaxy; Thermodynamics; Optics","score_opus":0.009496427000875293,"score_gpt":0.197668921338894,"score_spread":0.1881724943380187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049182449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9477021,0.0012599889,0.03896585,0.001331084,0.00006433623,0.000044957083,0.00021108743,0.00036530214,0.010055356],"genre_scores_gemma":[0.9949366,0.00044237255,0.002783523,0.000052478787,0.00004586694,0.00003973304,0.00005357205,0.000060232844,0.0015856088],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999343,0.000015322383,0.000002132981,0.0000134023,0.000009656777,0.000025112688],"domain_scores_gemma":[0.9996991,0.00010730923,0.00006612328,0.000036260597,0.000029449706,0.00006182317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032908336,0.0006835203,0.00045101237,0.0006081159,0.0006642143,0.0011970908,0.0016823602,0.0011461665,0.00088575634],"category_scores_gemma":[0.0009952983,0.0003383726,0.0007763592,0.00042964035,0.0015025996,0.0014039383,0.0009122139,0.00047096197,0.0002588703],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000058117428,0.000028369885,0.0066813817,0.000040632945,0.00004320704,0.00015546504,0.00020621852,0.9460139,0.00281982,0.04138427,0.0006762342,0.0018923163],"study_design_scores_gemma":[0.00003998655,0.000022541588,0.0031546575,0.000008261171,0.00002283699,0.000040036382,0.000054674994,0.969949,0.00034698684,0.025753979,0.00058832753,0.000018710636],"about_ca_topic_score_codex":0.014785706,"about_ca_topic_score_gemma":0.006592357,"teacher_disagreement_score":0.014785706,"about_ca_system_score_codex":0.0014005624,"about_ca_system_score_gemma":0.0006301738,"threshold_uncertainty_score":0.029399276},"labels":[],"label_agreement":null},{"id":"W2049229372","doi":"10.1086/521048","title":"SN 2001em: No Jet-driven Gamma-Ray Burst Event","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Very-long-baseline interferometry; Ejecta; Supernova; Proper motion; Gamma-ray burst; Jet (fluid); Event (particle physics); Relativistic beaming","score_opus":0.010365096012820667,"score_gpt":0.24427770617392758,"score_spread":0.2339126101611069,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049229372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9880001,0.0004075937,0.0010840987,0.000121082056,0.00010730448,0.000048567446,0.0025259,0.00015551277,0.007549839],"genre_scores_gemma":[0.98249775,0.00019257751,0.0016070863,0.00025651464,0.00008662411,0.00003016205,0.01150206,0.00005379444,0.0037734688],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998259,0.000013000617,0.000022444765,0.000045229288,0.00004637903,0.000047175934],"domain_scores_gemma":[0.999548,0.000044506356,0.000108879154,0.00007959991,0.00008984917,0.00012915228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003750667,0.00034451458,0.00038787766,0.00058333075,0.00047686667,0.00063907204,0.00031443196,0.0005114478,0.003283754],"category_scores_gemma":[0.0007774063,0.00011494762,0.0002469311,0.0003162252,0.00017528802,0.00031451412,0.0007157919,0.00042543397,0.00084321864],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026388802,0.0006349311,0.8756383,0.00028378685,0.00031562155,0.008976296,0.0003174206,0.00043133105,0.03317822,0.0017075621,0.0067126113,0.069165],"study_design_scores_gemma":[0.000120980694,0.00093932496,0.92094177,0.000044669854,0.00008609387,0.027611028,0.00017975259,0.00095469435,0.010071069,0.00071559334,0.038290016,0.0000451],"about_ca_topic_score_codex":0.0014522563,"about_ca_topic_score_gemma":0.0037938266,"teacher_disagreement_score":0.003283754,"about_ca_system_score_codex":0.0001643772,"about_ca_system_score_gemma":0.00021830013,"threshold_uncertainty_score":0.010985315},"labels":[],"label_agreement":null},{"id":"W2049276232","doi":"10.1086/430343","title":"The Magnetic Properties of an L Dwarf Derived from Simultaneous Radio, X‐Ray, and Hα Observations","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University","funders":"","keywords":"Physics; Astrophysics; Stars; Proper motion; Astronomy; Magnetic field; Rotation period; Luminosity; Circular polarization; Galaxy","score_opus":0.01657551169371936,"score_gpt":0.20759185414170658,"score_spread":0.1910163424479872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049276232","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99871767,0.00006434935,0.00031276414,0.000010260324,0.0000025734437,0.000002987212,0.00020719478,0.000020944519,0.00066118775],"genre_scores_gemma":[0.99881727,0.000030220039,0.0005480694,0.000014499664,0.000004738502,0.0000020830935,0.0003608044,0.000004985919,0.00021732773],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993944,0.000004890669,0.000004902455,0.000021815837,0.000016902708,0.000012041634],"domain_scores_gemma":[0.99969184,0.000040183564,0.00008627543,0.000024126986,0.00005653356,0.00010115326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015989988,0.00015580753,0.00014651788,0.0004378097,0.00027439345,0.00040066396,0.0001661994,0.00022800635,0.00048462942],"category_scores_gemma":[0.00035631988,0.0001130391,0.000110125584,0.00029449182,0.00016951821,0.00016208984,0.00022479285,0.00014890208,0.00033788456],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042262967,0.00007088797,0.61260504,0.00007070034,0.000029824845,0.0010387308,0.00059300894,0.00026051243,0.37126637,0.00009118495,0.00029471965,0.013256344],"study_design_scores_gemma":[0.000014461597,0.00020990442,0.98136234,0.000008389197,0.000021671036,0.0015053597,0.00027298147,0.00085376087,0.0143264895,0.00008386625,0.0013301219,0.000010598144],"about_ca_topic_score_codex":0.0018024688,"about_ca_topic_score_gemma":0.0039921873,"teacher_disagreement_score":0.0018024688,"about_ca_system_score_codex":0.00017793268,"about_ca_system_score_gemma":0.000125082,"threshold_uncertainty_score":0.003583908},"labels":[],"label_agreement":null},{"id":"W2049276958","doi":"10.1088/0004-637x/729/2/133","title":"STAR FORMATION EFFICIENCIES AND LIFETIMES OF GIANT MOLECULAR CLOUDS IN THE MILKY WAY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":376,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Star formation; Milky Way; Molecular cloud; Stars; Star cluster; Giant star; O-type star; Protostar","score_opus":0.012862195929638427,"score_gpt":0.21965833873548524,"score_spread":0.20679614280584682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049276958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99975604,0.000048213304,0.000022333388,0.000003311363,1.9266432e-7,5.0831596e-7,0.00008109251,0.0000018942435,0.00008639748],"genre_scores_gemma":[0.99938834,0.000054308122,0.000055672725,0.0000029834023,0.0000011648461,0.0000015972994,0.0004050335,0.000003048245,0.000087792716],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998331,0.000020105443,0.000013152479,0.000053643053,0.000026885331,0.000053055268],"domain_scores_gemma":[0.9984988,0.0003337136,0.00069591095,0.00013672584,0.00008940809,0.0002453765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043794245,0.00015540012,0.00024456697,0.0016151883,0.00019853505,0.00073977036,0.00031836904,0.00025748546,0.0006320827],"category_scores_gemma":[0.0026996213,0.00017431016,0.00031685564,0.0010324607,0.00028764937,0.0005571109,0.0006586469,0.00016218399,0.00017362193],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006647036,0.000011622442,0.9942972,0.000009847719,0.00006552983,0.00004346082,0.00025698598,0.0009829883,0.0018470658,0.00017895535,0.000050433708,0.002189546],"study_design_scores_gemma":[0.000003002376,0.000017172446,0.99824476,0.0000032964335,0.000014610192,0.00007721034,0.0001029563,0.00089129596,0.0003825458,0.00008928907,0.00017011816,0.0000036884908],"about_ca_topic_score_codex":0.006037066,"about_ca_topic_score_gemma":0.0068883104,"teacher_disagreement_score":0.006037066,"about_ca_system_score_codex":0.0005384283,"about_ca_system_score_gemma":0.00016999086,"threshold_uncertainty_score":0.012003839},"labels":[],"label_agreement":null},{"id":"W2049489325","doi":"10.1086/309128","title":"The Spatial Distribution of Atomic Carbon Emission in the Giant Molecular Cloud NGC 604‐2","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Molecular cloud; Astrophysics; Physics; Atomic carbon; Galaxy; Stars; James Clerk Maxwell Telescope; Star formation; H II region; Dissociation (chemistry); Photodissociation; Line (geometry); Emission spectrum; Astronomy; Spectral line; Chemistry; Hydrogen","score_opus":0.004360072971166733,"score_gpt":0.21770276253130033,"score_spread":0.2133426895601336,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049489325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99961144,0.000016319325,0.000031048778,0.000005992927,4.350969e-7,8.1269826e-7,0.00006209273,0.0000048334787,0.00026687994],"genre_scores_gemma":[0.9995314,0.000017758031,0.000097790165,0.0000046917435,0.0000015520909,0.0000017137177,0.00020335516,0.0000021736803,0.00013960742],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993885,0.000003067256,0.0000021583292,0.000015905198,0.000015064916,0.000024984594],"domain_scores_gemma":[0.999848,0.000014052116,0.00004803319,0.0000112595035,0.000024901497,0.000053667747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000069966845,0.00015468252,0.00013940857,0.00073662784,0.00032144756,0.00028336418,0.00018943325,0.00018398497,0.0008736665],"category_scores_gemma":[0.00020557376,0.0001287779,0.00008975523,0.0005045978,0.00017893377,0.00013993491,0.00034543476,0.000100724756,0.00016593702],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022303738,0.00004690041,0.76357615,0.00002966201,0.00004792333,0.0004667092,0.0006794042,0.0007116127,0.22548987,0.0002582823,0.00034130362,0.008129039],"study_design_scores_gemma":[0.00000825077,0.000019876326,0.9965689,0.0000030247934,0.000008965936,0.00011371559,0.000104921484,0.0005839064,0.0021084228,0.000038134585,0.00043828288,0.0000035956775],"about_ca_topic_score_codex":0.017899254,"about_ca_topic_score_gemma":0.028803675,"teacher_disagreement_score":0.017899254,"about_ca_system_score_codex":0.00044298614,"about_ca_system_score_gemma":0.00012657193,"threshold_uncertainty_score":0.035590112},"labels":[],"label_agreement":null},{"id":"W2049490959","doi":"10.1086/321369","title":"The MACHO Project LMC Variable Star Inventory. X. The R Coronae Borealis Stars","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Variable star; Stars; Star (game theory); Stellar evolution; Universe","score_opus":0.01575481084156826,"score_gpt":0.23898485105936723,"score_spread":0.22323004021779896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049490959","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0071796253,0.0018086683,0.009280401,0.0014815188,0.00028534036,0.00021122246,0.8714507,0.021153118,0.087149486],"genre_scores_gemma":[0.012467705,0.00084048207,0.017990163,0.00024498714,0.00015038463,0.00015193544,0.9404847,0.0027508666,0.024918817],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9993612,0.00007068671,0.000056985114,0.00012076677,0.00028047102,0.00010997931],"domain_scores_gemma":[0.9975879,0.0001651446,0.00035288616,0.00072590826,0.0006420087,0.0005261043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015821981,0.00096226076,0.00081480294,0.004166988,0.0009823649,0.0034772079,0.0014786243,0.0007940317,0.054070745],"category_scores_gemma":[0.003202389,0.0005116272,0.00049798045,0.0064928723,0.00029428749,0.0029483025,0.0029415635,0.00081497256,0.053563252],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039359005,0.00007542514,0.0069725094,0.0003955015,0.000049749484,0.000059806225,0.00015781159,0.000594505,0.0017967877,0.010100819,0.8744975,0.104906045],"study_design_scores_gemma":[0.000064733125,0.00002880641,0.009883609,0.00008337668,0.000023096809,0.000069449175,0.0000804169,0.000997874,0.00093159266,0.0052453117,0.9825713,0.00002051201],"about_ca_topic_score_codex":0.03193126,"about_ca_topic_score_gemma":0.02232934,"teacher_disagreement_score":0.054070745,"about_ca_system_score_codex":0.0010120296,"about_ca_system_score_gemma":0.00214627,"threshold_uncertainty_score":0.18088466},"labels":[],"label_agreement":null},{"id":"W2049532750","doi":"10.1086/586690","title":"Stellar Wind Variations during the X‐Ray High and Low States of Cygnus X‐11,2","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; National Science Foundation; Ministerio de Economía y Competitividad; University of Toronto; National Aeronautics and Space Administration; Space Telescope Science Institute","keywords":"Physics; Supergiant; Astrophysics; Stars; Ionization; Photoionization; Astronomy; Emission spectrum; Spectral line; Ion","score_opus":0.007577572451175061,"score_gpt":0.1964439574153783,"score_spread":0.18886638496420322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049532750","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952066,0.000015822357,0.00002386693,0.000004616629,0.0000010314541,0.000001772626,0.00014957604,0.000002637394,0.0002798854],"genre_scores_gemma":[0.9989496,0.000011135283,0.00005092742,0.00000478639,0.000002756389,0.000003186022,0.0006706933,0.0000020132716,0.00030491652],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995875,0.000004497357,0.0000027533933,0.00001169375,0.0000074322693,0.000014908484],"domain_scores_gemma":[0.9998349,0.000024366802,0.000053614815,0.0000096145495,0.00002517085,0.000052309933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001077103,0.00012432621,0.00009543702,0.00040032878,0.00026881992,0.00037320243,0.00010114652,0.00020494104,0.001089114],"category_scores_gemma":[0.00030243633,0.0000573195,0.00009525537,0.00022258332,0.00013799172,0.0001335966,0.00022541506,0.00021833114,0.00023364388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030972605,0.000076231845,0.9829375,0.000010394315,0.000018061432,0.00013914617,0.00021127466,0.00034659,0.012461313,0.000067036,0.00016922536,0.0032535593],"study_design_scores_gemma":[0.0000018073955,0.0000227033,0.9993247,8.771591e-7,0.0000020291425,0.00003212371,0.00003952177,0.00015142572,0.00029027596,0.000006280313,0.00012713681,0.0000011806809],"about_ca_topic_score_codex":0.0057067755,"about_ca_topic_score_gemma":0.01493888,"teacher_disagreement_score":0.0057067755,"about_ca_system_score_codex":0.00028941873,"about_ca_system_score_gemma":0.00009209369,"threshold_uncertainty_score":0.011347115},"labels":[],"label_agreement":null},{"id":"W2049648180","doi":"10.1088/0004-637x/764/2/162","title":"THERMAL PLASMA IN THE GIANT LOBES OF THE RADIO GALAXY CENTAURUS A","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Faraday effect; Radio galaxy; Plasma; Thermal; Centaurus A; Mean kinetic temperature; Magnetic field","score_opus":0.00585103377320296,"score_gpt":0.19013177748141102,"score_spread":0.18428074370820807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049648180","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987795,0.00026145452,0.00011407788,0.000014031944,0.0000026283856,0.0000020950279,0.00010956563,0.000017484736,0.0006992941],"genre_scores_gemma":[0.99945146,0.00007768761,0.00010181552,0.000012270731,0.000008361665,0.0000020495304,0.00019861701,0.0000041243034,0.00014357935],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993765,0.000007237998,0.0000027743317,0.000020100584,0.0000126867135,0.00001965264],"domain_scores_gemma":[0.9998566,0.00002140286,0.000052077667,0.000014982413,0.000014111124,0.000040816165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001067069,0.00016490248,0.00014675446,0.0012132574,0.0003849405,0.0007600819,0.00020498832,0.00020148944,0.0005372541],"category_scores_gemma":[0.00025096774,0.0001492781,0.00013612575,0.00060347957,0.00040948158,0.00021100274,0.00060698704,0.00014370603,0.00019620472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006012568,0.00009109926,0.56464744,0.00010628169,0.00009877204,0.0024169863,0.0028062556,0.0005493025,0.40239537,0.00044551626,0.00063741446,0.025204424],"study_design_scores_gemma":[0.000004947127,0.00004646423,0.99562645,0.0000044565245,0.000013295808,0.0004422101,0.00025423893,0.00023733746,0.0026578156,0.00007551562,0.0006315156,0.0000057694647],"about_ca_topic_score_codex":0.0038027598,"about_ca_topic_score_gemma":0.0036873466,"teacher_disagreement_score":0.0038027598,"about_ca_system_score_codex":0.00026725978,"about_ca_system_score_gemma":0.00007429378,"threshold_uncertainty_score":0.007561207},"labels":[],"label_agreement":null},{"id":"W2049655293","doi":"10.1086/509567","title":"Very High Energy Observations of Gamma‐Ray Burst Locations with the Whipple Telescope","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Gamma-ray burst; Afterglow; Telescope; Flare; High energy; Spectral energy distribution","score_opus":0.011972645262756819,"score_gpt":0.2141571911334637,"score_spread":0.2021845458707069,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049655293","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9643378,0.0017331232,0.010707646,0.00016233277,0.000057316684,0.00006205034,0.0039688875,0.0004619183,0.018508848],"genre_scores_gemma":[0.98881406,0.00052765844,0.0053706737,0.00007652804,0.000025512158,0.000017363005,0.0028970595,0.000025236557,0.0022459694],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996817,0.000024241022,0.000028175376,0.000076440636,0.000119913966,0.00006960496],"domain_scores_gemma":[0.99818295,0.0004322078,0.0005655624,0.00027525722,0.00026455958,0.00027948897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068969664,0.00027650435,0.00027984896,0.0013085777,0.0005166496,0.0006502759,0.00033011462,0.0003452968,0.0026398068],"category_scores_gemma":[0.00139213,0.00021823749,0.00028120494,0.00090318214,0.00032786143,0.0004550831,0.0011539167,0.0006327946,0.0007995329],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024988715,0.00006675993,0.82968336,0.00021181046,0.00012758726,0.001461782,0.0008323615,0.00051587465,0.07981231,0.0010806202,0.0031684441,0.08278923],"study_design_scores_gemma":[0.000009098143,0.00013631431,0.97567296,0.000026036367,0.000033553533,0.0020874545,0.0001733957,0.00035581033,0.009166839,0.0004552559,0.01185542,0.000027842865],"about_ca_topic_score_codex":0.0013374685,"about_ca_topic_score_gemma":0.003009648,"teacher_disagreement_score":0.0026398068,"about_ca_system_score_codex":0.00019868407,"about_ca_system_score_gemma":0.00016795564,"threshold_uncertainty_score":0.008831024},"labels":[],"label_agreement":null},{"id":"W2049845141","doi":"10.1088/0004-637x/747/2/119","title":"A 2.15 hr ORBITAL PERIOD FOR THE LOW-MASS X-RAY BINARY XB 1832-330 IN THE GLOBULAR CLUSTER NGC 6652","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Light curve; Orbital period; Amplitude; Stars; Binary number; Binary star; Magnitude (astronomy); Cluster (spacecraft)","score_opus":0.01391389921321538,"score_gpt":0.24335253874695642,"score_spread":0.22943863953374105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049845141","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99871445,0.000062182065,0.00014974058,0.000022661776,0.0000043594387,0.0000038838193,0.0002035132,0.000017354854,0.00082187844],"genre_scores_gemma":[0.9991086,0.000020310628,0.00030322015,0.0000073138694,0.0000046137498,0.0000024569754,0.0003259182,0.000003052761,0.00022445622],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999455,0.000004711708,0.0000026846346,0.0000200027,0.000010755829,0.000016243588],"domain_scores_gemma":[0.9998596,0.000013084019,0.000054600096,0.000015263688,0.000012070311,0.000045382298],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015108414,0.00017402037,0.0001490707,0.000557996,0.00049551565,0.00042525094,0.00014436981,0.0003251062,0.0015692674],"category_scores_gemma":[0.0002889638,0.00012320564,0.00013952493,0.0004501171,0.00013244967,0.00014172102,0.00028847274,0.00015669044,0.00032943368],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011744493,0.00010807441,0.83956254,0.0001293917,0.00004759827,0.0019641134,0.0005568675,0.0009707945,0.13631508,0.00042047177,0.0010762824,0.01767432],"study_design_scores_gemma":[0.000008898872,0.000061740306,0.99801564,0.000004698355,0.000010889127,0.00018042621,0.00006566453,0.00054135453,0.00074219244,0.0000245245,0.00033999654,0.0000038369576],"about_ca_topic_score_codex":0.0055177035,"about_ca_topic_score_gemma":0.016756155,"teacher_disagreement_score":0.0055177035,"about_ca_system_score_codex":0.0003000271,"about_ca_system_score_gemma":0.00016600665,"threshold_uncertainty_score":0.010971129},"labels":[],"label_agreement":null},{"id":"W2049857179","doi":"10.1088/0004-637x/791/1/27","title":"THE IDENTIFICATION OF FILAMENTS ON FAR-INFRARED AND SUBMILLIMITER IMAGES: MORPHOLOGY, PHYSICAL CONDITIONS AND RELATION WITH STAR FORMATION OF FILAMENTARY STRUCTURE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":142,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Science and Technology Facilities Council; Ministerio de Ciencia e Innovación; European Commission; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Star formation; Molecular cloud; Longitude; Stars; Range (aeronautics); Stability (learning theory); Gravitational collapse; Protein filament; Star (game theory)","score_opus":0.005598785654077328,"score_gpt":0.2238653442655062,"score_spread":0.21826655861142888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049857179","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99417406,0.000095740885,0.004521921,0.000017861888,0.0000019648594,0.00001136814,0.00031106756,0.0000686297,0.00079720106],"genre_scores_gemma":[0.99266875,0.000040247058,0.006554572,0.0000060776665,0.0000041662415,0.0000056143595,0.00055542105,0.000011899458,0.00015340668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993324,0.000007895315,0.0000038924068,0.000021378753,0.000013512556,0.000020053969],"domain_scores_gemma":[0.9997137,0.00007658376,0.000092842296,0.000031507097,0.000041110565,0.00004426541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018396463,0.00014315116,0.00011199708,0.00078756275,0.00019623204,0.00043121344,0.00017579601,0.00025721727,0.00073928083],"category_scores_gemma":[0.00064349733,0.00012404911,0.00017515302,0.00041019634,0.00012902742,0.00030631083,0.00021906347,0.0001268929,0.00018971146],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020992487,0.000084165775,0.81331277,0.00007439138,0.00008813905,0.0003533873,0.00030356643,0.009553158,0.11869311,0.0006217277,0.0006389325,0.05606675],"study_design_scores_gemma":[0.000005375945,0.000018183555,0.9694111,0.00000935108,0.000020216428,0.00019900677,0.00008396091,0.021751791,0.007927347,0.00022660563,0.0003393908,0.000007666752],"about_ca_topic_score_codex":0.002554567,"about_ca_topic_score_gemma":0.0048905965,"teacher_disagreement_score":0.002554567,"about_ca_system_score_codex":0.0002466492,"about_ca_system_score_gemma":0.00008410408,"threshold_uncertainty_score":0.005079448},"labels":[],"label_agreement":null},{"id":"W2049873521","doi":"10.1086/308881","title":"A Search for Flux Density Variations in 24 Compact Radio Sources in M82","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Flux (metallurgy); Luminosity; Supernova; Galaxy; Astronomy; Population","score_opus":0.019072949216953395,"score_gpt":0.3234488651041706,"score_spread":0.3043759158872172,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049873521","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995254,0.00006910158,0.00015198223,0.00000878022,6.019937e-7,0.0000029347914,0.00008631686,0.00001131814,0.00014361955],"genre_scores_gemma":[0.9987545,0.00007193003,0.0004690165,0.000009427889,0.000012813335,0.00000830069,0.00044160458,0.0000051436255,0.00022729559],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986887,0.000019400926,0.000008016755,0.000039482773,0.000033572695,0.000030643736],"domain_scores_gemma":[0.9992347,0.00013193695,0.0003399447,0.00008216187,0.000094314644,0.00011690415],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029062238,0.00027738968,0.00023652405,0.0015294672,0.00042255982,0.00049065717,0.0002865247,0.00036570066,0.0007216322],"category_scores_gemma":[0.00092768326,0.0002784581,0.00012374335,0.00096455903,0.00023742241,0.00026169734,0.00037876627,0.0001971822,0.0003838591],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022553536,0.00015029337,0.9231341,0.00002700024,0.00005743316,0.00053638045,0.00081902096,0.00042766752,0.05031062,0.000109185814,0.00021916015,0.023983449],"study_design_scores_gemma":[0.000004890384,0.00008461918,0.998309,0.000001880193,0.000012036776,0.00020069063,0.000051198393,0.00025228845,0.00075772905,0.000021523518,0.0003002028,0.000003942424],"about_ca_topic_score_codex":0.0022050752,"about_ca_topic_score_gemma":0.0046316064,"teacher_disagreement_score":0.0022050752,"about_ca_system_score_codex":0.00020491172,"about_ca_system_score_gemma":0.00011579715,"threshold_uncertainty_score":0.004384458},"labels":[],"label_agreement":null},{"id":"W2049963427","doi":"10.1086/375160","title":"The Impact of Ionizing Stars on the Diffuse Interstellar Medium: A Swept‐up Shell and Ionized Halo around the W4 Chimney/Superbubble","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; University of Waterloo","funders":"","keywords":"Superbubble; Physics; Astrophysics; Galactic plane; Interstellar medium; Galaxy; Astronomy; Supernova; Halo; Galactic halo; Galactic corona; Cosmic dust; Milky Way; Ionization","score_opus":0.014703329112190643,"score_gpt":0.2481326064260547,"score_spread":0.23342927731386406,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049963427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907124,0.00004469899,0.000069401445,0.0000082107435,6.82537e-7,0.0000016387725,0.000021551521,0.0000057845814,0.00077658653],"genre_scores_gemma":[0.99954885,0.00001985268,0.00009178762,0.00000586613,9.101358e-7,8.9684187e-7,0.00005730594,0.0000036412653,0.0002708985],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996245,0.0000023498026,0.0000010670725,0.000007774115,0.000008524136,0.000017776945],"domain_scores_gemma":[0.99989414,0.0000065638555,0.000029629397,0.0000059432314,0.000008231616,0.000055393335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000053259326,0.00020598601,0.0001290535,0.0006742859,0.00045638203,0.00048821047,0.00028853465,0.00013724754,0.001653491],"category_scores_gemma":[0.00010972736,0.00015052708,0.00012936522,0.000343328,0.0004545908,0.00024539803,0.000859921,0.00017227103,0.0002678327],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006290357,0.000085931555,0.6889168,0.000051469393,0.00009734043,0.004798299,0.0008130753,0.001447876,0.29195264,0.0011765772,0.0005317375,0.0094992295],"study_design_scores_gemma":[0.000011523558,0.00008817484,0.98998123,0.000005125793,0.000015855623,0.00087022263,0.00064577535,0.0014603281,0.0056056324,0.00025970562,0.0010471656,0.000009361763],"about_ca_topic_score_codex":0.0069848485,"about_ca_topic_score_gemma":0.008290128,"teacher_disagreement_score":0.0069848485,"about_ca_system_score_codex":0.00036132472,"about_ca_system_score_gemma":0.00015134325,"threshold_uncertainty_score":0.013888419},"labels":[],"label_agreement":null},{"id":"W2049967503","doi":"10.1088/0004-637x/736/2/140","title":"A SYSTEMATIC SEARCH FOR COROTATING INTERACTION REGIONS IN APPARENTLY SINGLE GALACTIC WOLF-RAYET STARS. II. A GLOBAL VIEW OF THE WIND VARIABILITY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec; Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Solar wind; Error analysis; Systematic error; Starspot; Spectral line","score_opus":0.036421328205080095,"score_gpt":0.2668348956270734,"score_spread":0.23041356742199331,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2049967503","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978935,0.0007609432,0.0006181111,0.000012371999,0.0000033329825,0.00001588822,0.00016739705,0.000024027357,0.0005044998],"genre_scores_gemma":[0.996968,0.00030751675,0.001689303,0.000022207118,0.000013924029,0.000013738337,0.00068544934,0.000012329384,0.0002876081],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962485,0.000035335775,0.000037111757,0.0001854705,0.000061987535,0.00005527226],"domain_scores_gemma":[0.9989017,0.00013506568,0.00045424709,0.00012086824,0.00011813039,0.0002699409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045254873,0.00034601288,0.00039525796,0.0031700234,0.00049398624,0.0006770578,0.00031560656,0.00035645493,0.0008271391],"category_scores_gemma":[0.00045907637,0.00019218423,0.0003703665,0.0015978386,0.00030786073,0.00043383203,0.0007663034,0.00023106873,0.00036950826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009029801,0.000027707356,0.93266624,0.000083399544,0.000067734254,0.0004899892,0.00023062956,0.00009806824,0.049141936,0.000051955256,0.00006690026,0.016985169],"study_design_scores_gemma":[0.000003571308,0.00014523935,0.99463403,0.000008152485,0.00005574949,0.001268824,0.00018782896,0.0001511756,0.002802242,0.00004383496,0.00069357717,0.000005713333],"about_ca_topic_score_codex":0.00043778116,"about_ca_topic_score_gemma":0.0014260747,"teacher_disagreement_score":0.0031700234,"about_ca_system_score_codex":0.00013734338,"about_ca_system_score_gemma":0.00019258064,"threshold_uncertainty_score":0.0027670264},"labels":[],"label_agreement":null},{"id":"W2050008113","doi":"10.1088/0004-637x/757/1/102","title":"WHAT DO DARK MATTER HALO PROPERTIES TELL US ABOUT THEIR MASS ASSEMBLY HISTORIES?","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Halo; Astrophysics; Physics; Accretion (finance); Dark matter; Dark matter halo; Galaxy; Galaxy formation and evolution; Cosmology; Substructure","score_opus":0.01003029025708524,"score_gpt":0.20043558571602701,"score_spread":0.19040529545894178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050008113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99206287,0.00061246846,0.0039058158,0.0005071297,0.000008119399,0.000010997937,0.0010214302,0.00006457586,0.0018066303],"genre_scores_gemma":[0.9977975,0.00036271082,0.0007847198,0.00006892897,0.000018648907,0.0000060040106,0.00060062046,0.0000501327,0.00031065778],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99960905,0.00012032129,0.000028636432,0.00012920931,0.00004338156,0.00006952727],"domain_scores_gemma":[0.9888849,0.0050063916,0.0028118473,0.0013116346,0.00072834647,0.0012568878],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024330183,0.00032876633,0.0007311309,0.0020937815,0.00055132795,0.0025257273,0.0008048801,0.0010732501,0.002231787],"category_scores_gemma":[0.025125224,0.000835335,0.0006412942,0.0015675201,0.0012917675,0.0046551763,0.0010554323,0.00071004994,0.00065708294],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019174005,0.000022683162,0.9611598,0.00008236332,0.00043216706,0.00009961013,0.00083673093,0.018197412,0.002332515,0.0036783663,0.0004938325,0.012472742],"study_design_scores_gemma":[0.00002374405,0.00006892798,0.940232,0.000043522567,0.00012003085,0.00016071355,0.00068091624,0.043757696,0.0014926816,0.012079173,0.0012595793,0.00008099402],"about_ca_topic_score_codex":0.007126515,"about_ca_topic_score_gemma":0.008844637,"teacher_disagreement_score":0.007126515,"about_ca_system_score_codex":0.00076553517,"about_ca_system_score_gemma":0.00028676057,"threshold_uncertainty_score":0.014170051},"labels":[],"label_agreement":null},{"id":"W2050152431","doi":"10.1086/524194","title":"Erratum: “Multiwavelength Mass Comparisons of the<i>z</i>∼ 0.3 CNOC Cluster Sample” (ApJ, 652, 232 [2006])","year":2008,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Victoria","funders":"","keywords":"Physics; Cluster (spacecraft); Astrophysics; Sample (material); Thermodynamics","score_opus":0.012371025314922549,"score_gpt":0.2477226738772265,"score_spread":0.23535164856230395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050152431","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0064030997,0.001953828,0.0010054692,0.060577225,0.8594434,0.00012246505,0.031731587,0.0016617383,0.037101183],"genre_scores_gemma":[0.041855536,0.004645046,0.008861303,0.06884434,0.059100702,0.0003042769,0.061338443,0.0035694146,0.751481],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987369,0.00008331891,0.0002502068,0.0001843135,0.00062496815,0.000120285695],"domain_scores_gemma":[0.99127126,0.0012492901,0.0005280583,0.0006393109,0.0058823638,0.00042971352],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012308172,0.0013340178,0.000979382,0.0037075556,0.0034094057,0.0019330105,0.0023856757,0.0020533176,0.051051],"category_scores_gemma":[0.01595772,0.0005700176,0.0006868643,0.0025066647,0.00075528,0.0013730746,0.0012620378,0.002544224,0.028651442],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036880956,0.000011496987,0.00032176348,0.0000434196,0.000004282742,0.00010166294,0.000017283252,0.000021935448,0.00009360298,0.00019335796,0.99550784,0.003646383],"study_design_scores_gemma":[0.000062396684,0.000049078808,0.019183094,0.00023111567,0.000057253,0.00040802878,0.00025878003,0.0002660054,0.0013518367,0.00080847164,0.97725505,0.000068928515],"about_ca_topic_score_codex":0.058365427,"about_ca_topic_score_gemma":0.094578244,"teacher_disagreement_score":0.058365427,"about_ca_system_score_codex":0.0028123318,"about_ca_system_score_gemma":0.0029846118,"threshold_uncertainty_score":0.17078257},"labels":[],"label_agreement":null},{"id":"W2050184593","doi":"10.1086/322276","title":"The Dynamics of Sinking Satellites around Disk Galaxies: A Poor Man’s Alternative to High‐Resolution Numerical Simulations","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":221,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Substructure; Population; Galaxy; Simple (philosophy); Dynamical systems theory; Galaxy formation and evolution; Set (abstract data type); Dynamical friction; Dynamical system (definition)","score_opus":0.008298114370176905,"score_gpt":0.23079912880016004,"score_spread":0.22250101442998313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050184593","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.27974302,0.00087239785,0.6934352,0.0015129347,0.00014263007,0.00017855031,0.0004715929,0.0019040771,0.021739613],"genre_scores_gemma":[0.85515255,0.000384368,0.1412741,0.00016757894,0.00006294143,0.00017281901,0.0001498385,0.00028250928,0.0023533776],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996867,0.00013456757,0.000016115255,0.00003049203,0.000098021614,0.00003404575],"domain_scores_gemma":[0.9974408,0.0011520135,0.00027072424,0.00075164466,0.00021511764,0.00016962473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00090481696,0.0005092123,0.0010531413,0.0005230819,0.0006648299,0.0013163985,0.0021934228,0.0010385984,0.0027413187],"category_scores_gemma":[0.005946439,0.0004938521,0.0005355584,0.0005703255,0.0012319161,0.0018582306,0.0016342812,0.0012627852,0.0006869393],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005472004,0.000053274078,0.0024995266,0.000050988685,0.00003885086,0.000080506456,0.00012494678,0.95728433,0.0022435416,0.030102788,0.0004540058,0.0070125763],"study_design_scores_gemma":[0.000013215672,0.0000072645835,0.00014173515,0.0000037081293,0.0000023039431,0.000007678287,0.0000075932708,0.9962657,0.00017764604,0.0029844302,0.00038397883,0.000004678466],"about_ca_topic_score_codex":0.011704179,"about_ca_topic_score_gemma":0.006724674,"teacher_disagreement_score":0.011704179,"about_ca_system_score_codex":0.0009984823,"about_ca_system_score_gemma":0.0008915565,"threshold_uncertainty_score":0.023272097},"labels":[],"label_agreement":null},{"id":"W2050186897","doi":"10.1086/382701","title":"H <sub>2</sub> Emission Nebulosity Associated with KH 15D","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Protein filament; Outflow; Emission spectrum; Subaru Telescope; Bipolar outflow; H II region","score_opus":0.008444598203242757,"score_gpt":0.23596947585244038,"score_spread":0.22752487764919763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050186897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975241,0.00008560058,0.000108224136,0.000024362893,0.000003432697,0.0000044296585,0.0001359089,0.000014814007,0.0020990854],"genre_scores_gemma":[0.99939287,0.000027855624,0.00016305326,0.000034946475,0.000004986499,0.0000025866732,0.00017781982,0.0000035746677,0.00019223349],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998932,0.0000031078491,0.000007954212,0.00003254273,0.000022387507,0.0000407137],"domain_scores_gemma":[0.9997373,0.000013996903,0.000114323375,0.000019048355,0.000021471653,0.000093826544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009205199,0.00012117401,0.0002370451,0.00069399585,0.0005045105,0.0005456029,0.00029096226,0.00019413243,0.0011802275],"category_scores_gemma":[0.00018128548,0.00013708431,0.00015404534,0.00044567042,0.00060908234,0.00016729679,0.000807172,0.00019778324,0.00022655012],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023957474,0.00005363206,0.91491306,0.00006677604,0.000065786306,0.0019175969,0.0005584795,0.00028317297,0.06923091,0.0006877905,0.00058371434,0.011399433],"study_design_scores_gemma":[0.000008553838,0.000035136178,0.9959208,0.0000074511477,0.000013263019,0.0010842495,0.00013175873,0.00011423797,0.001483831,0.0000875649,0.0011084864,0.00000456883],"about_ca_topic_score_codex":0.006938681,"about_ca_topic_score_gemma":0.014329587,"teacher_disagreement_score":0.006938681,"about_ca_system_score_codex":0.000753289,"about_ca_system_score_gemma":0.0002275095,"threshold_uncertainty_score":0.0137966275},"labels":[],"label_agreement":null},{"id":"W2050188062","doi":"10.1088/0004-637x/801/2/72","title":"THE<i>HERSCHEL</i>COMPREHENSIVE (U)LIRG EMISSION SURVEY (HERCULES): CO LADDERS, FINE STRUCTURE LINES, AND NEUTRAL GAS COOLING","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":176,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"U.S. Naval Research Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Naval Research; Centre National de la Recherche Scientifique; Università degli Studi di Padova; Centre National d’Etudes Spatiales; Cardiff University; University of Sussex; National Aeronautics and Space Administration; California Institute of Technology; University of Lethbridge; Imperial College London; Canadian Space Agency; UK Space Agency","keywords":"Luminous infrared galaxy; Infrared; Luminosity; Galaxy; Emission spectrum; Line (geometry); Infrared astronomy; Active galactic nucleus","score_opus":0.017850938521326652,"score_gpt":0.24292107037621244,"score_spread":0.22507013185488578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050188062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6288278,0.0059587643,0.008453816,0.0015410284,0.00009404831,0.00040079353,0.24188045,0.004685001,0.10815829],"genre_scores_gemma":[0.794702,0.0020747632,0.027232643,0.0008777479,0.00024197003,0.00028736223,0.16248843,0.00045337543,0.011641675],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997514,0.000024013118,0.000011132324,0.00007457424,0.000070263646,0.00006867926],"domain_scores_gemma":[0.99942064,0.000026528465,0.00026289042,0.00008656426,0.000056748246,0.00014662268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005957973,0.00062337256,0.0003551223,0.0025130194,0.00047577877,0.00067827484,0.00051569415,0.00031950776,0.0056200526],"category_scores_gemma":[0.00047657927,0.00014989071,0.0001995095,0.0022706403,0.00030615958,0.00049095915,0.0011857378,0.00033470048,0.0020935414],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023471049,0.00013419637,0.68694854,0.00038369754,0.00021187852,0.00023308281,0.00048700045,0.0011275788,0.023319416,0.005115938,0.1785732,0.103230804],"study_design_scores_gemma":[0.000033389504,0.000030015051,0.895481,0.000047694797,0.000040094354,0.00019074135,0.000102787686,0.00052721053,0.003428474,0.0006244263,0.099473156,0.000021075051],"about_ca_topic_score_codex":0.019712321,"about_ca_topic_score_gemma":0.040701583,"teacher_disagreement_score":0.019712321,"about_ca_system_score_codex":0.00077211834,"about_ca_system_score_gemma":0.00055611087,"threshold_uncertainty_score":0.03919518},"labels":[],"label_agreement":null},{"id":"W2050200918","doi":"10.1086/527281","title":"A Global Probe of Cosmic Magnetic Fields to High Redshifts","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Redshift; Faraday effect; Magnetic field; Quasar; Galaxy; Universe; COSMIC cancer database; Radio galaxy; Field (mathematics)","score_opus":0.0070958392888228455,"score_gpt":0.23323158713042955,"score_spread":0.2261357478416067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050200918","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921788,0.00015404887,0.0028926136,0.00005854373,0.0000034547866,0.0000031267434,0.00057414814,0.00006292991,0.0040723183],"genre_scores_gemma":[0.9986053,0.00007544497,0.00056470203,0.000021174235,0.000013384871,0.0000030848594,0.00033836815,0.000013270656,0.00036537382],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985063,0.00002148433,0.0000042013576,0.000060789505,0.00002119591,0.000041678457],"domain_scores_gemma":[0.9988527,0.00021420691,0.0004598943,0.00016436522,0.0000843105,0.00022452718],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030704236,0.00025986464,0.00031516427,0.0014676998,0.0002025508,0.0006861263,0.00014913554,0.00021593069,0.002059457],"category_scores_gemma":[0.0013379686,0.00013226402,0.0001987284,0.0011729666,0.00035094257,0.0006233595,0.00090186903,0.00041490898,0.00028255783],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014328177,0.000045950645,0.91902584,0.000067869856,0.00017137695,0.00015987133,0.0010932445,0.0024270792,0.03737115,0.0050178226,0.00070909504,0.033767436],"study_design_scores_gemma":[0.0000020218172,0.000019717045,0.9970625,0.000002888991,0.00001567716,0.00005945441,0.000082087,0.000553693,0.0007637499,0.00047331897,0.0009614266,0.000003270972],"about_ca_topic_score_codex":0.0012637333,"about_ca_topic_score_gemma":0.0016440739,"teacher_disagreement_score":0.002059457,"about_ca_system_score_codex":0.00019312844,"about_ca_system_score_gemma":0.00007238089,"threshold_uncertainty_score":0.0068895817},"labels":[],"label_agreement":null},{"id":"W2050285721","doi":"10.1086/430405","title":"An<i>HST</i>Search for Supernovae Accompanying X‐Ray Flashes","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Supernova; Redshift; Hubble space telescope; Pair-instability supernova; Spectroscopy; Cosmology; Type (biology); Light curve","score_opus":0.020224436408163363,"score_gpt":0.27414822421402874,"score_spread":0.2539237878058654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050285721","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99087673,0.00027349536,0.00061945966,0.00023142021,0.00002673697,0.00004540173,0.0016960114,0.00010545744,0.006125313],"genre_scores_gemma":[0.9901751,0.00037765174,0.0023687812,0.00044635896,0.00009387824,0.000016082911,0.0036221615,0.00001573143,0.0028843216],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999936,0.0000047888147,0.0000063415287,0.000010666693,0.00002184376,0.000020400877],"domain_scores_gemma":[0.99955815,0.0000511159,0.00011522717,0.000029495804,0.00006360815,0.00018232882],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018999765,0.00027587658,0.00017475034,0.0013857002,0.00048287527,0.00050616503,0.00021464794,0.0004033202,0.00500795],"category_scores_gemma":[0.00028394884,0.000087452616,0.00025848555,0.0007138892,0.00021894569,0.00021119716,0.00027816222,0.0002274403,0.0007424265],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002209018,0.00020005349,0.86135465,0.000104141436,0.00015901707,0.0030499585,0.00018200716,0.0002867121,0.11155367,0.00045519133,0.0023853802,0.02004831],"study_design_scores_gemma":[0.0000259766,0.000342149,0.97297937,0.000012454381,0.00006574659,0.0037935537,0.00017208245,0.00041846535,0.015968198,0.00025603533,0.005951731,0.000014113955],"about_ca_topic_score_codex":0.0028612781,"about_ca_topic_score_gemma":0.0077638747,"teacher_disagreement_score":0.00500795,"about_ca_system_score_codex":0.00012894193,"about_ca_system_score_gemma":0.00017014946,"threshold_uncertainty_score":0.016753256},"labels":[],"label_agreement":null},{"id":"W2050286498","doi":"10.1086/321508","title":"The Structure of Self‐gravitating Polytropic Systems with<i>n</i>around 5","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Statistical Mechanics and Entropy","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Polytropic process; Polytrope; Nonlinear system; Stellar structure; Stability (learning theory); Duality (order theory); Poisson distribution","score_opus":0.005619057781181184,"score_gpt":0.2218555897203576,"score_spread":0.2162365319391764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050286498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917441,0.00013647135,0.0045325328,0.000097853095,0.000004600205,0.000008632273,0.000020384605,0.00002821353,0.0034270533],"genre_scores_gemma":[0.99729365,0.000059130354,0.001873264,0.000019104184,0.000009963974,0.000010182496,0.000043865282,0.000008674685,0.000682001],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999027,0.000014794698,0.0000034702582,0.000022205935,0.000018539673,0.000038272636],"domain_scores_gemma":[0.9993573,0.000089864676,0.0002802718,0.000046102552,0.00006723201,0.00015920063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016144894,0.00018806227,0.0002506748,0.00073139503,0.0007959821,0.00075361924,0.0005585574,0.0004609397,0.0015918433],"category_scores_gemma":[0.00082701223,0.00021547268,0.00024114357,0.0004036714,0.0015959227,0.000593023,0.00086010207,0.00038627232,0.00018422495],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004334717,0.0002880573,0.09276668,0.00021620488,0.0001804554,0.0019953926,0.0026820987,0.29454482,0.08905527,0.49038866,0.003521948,0.023926912],"study_design_scores_gemma":[0.000059809932,0.00017865366,0.06284164,0.000024736622,0.000045610086,0.00062599505,0.00053394685,0.8038581,0.007335062,0.120947845,0.0034822237,0.000066383865],"about_ca_topic_score_codex":0.0015603267,"about_ca_topic_score_gemma":0.001019012,"teacher_disagreement_score":0.0015918433,"about_ca_system_score_codex":0.0006216259,"about_ca_system_score_gemma":0.0004258186,"threshold_uncertainty_score":0.005325198},"labels":[],"label_agreement":null},{"id":"W2050306440","doi":"10.1086/308538","title":"Betelgeuse and Its Variations","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Astronomy","score_opus":0.009844229899981311,"score_gpt":0.21847759120884114,"score_spread":0.20863336130885982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050306440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9899974,0.0014656027,0.00011758055,0.00018570361,0.000011410125,0.0000050159492,0.00032371166,0.000012796782,0.007880769],"genre_scores_gemma":[0.99694866,0.00042631538,0.00010134045,0.000042538373,0.0000105863755,0.0000029535,0.00022122615,0.0000058126507,0.0022405973],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983895,0.000012650812,0.0000043297973,0.000050684248,0.000043440563,0.000050020528],"domain_scores_gemma":[0.99980205,0.000018916093,0.00005903975,0.000009597708,0.000028093387,0.00008234772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010047237,0.00019579842,0.00018920022,0.0016904798,0.0006963129,0.0005689261,0.00027015753,0.00029137533,0.0019462651],"category_scores_gemma":[0.00068070384,0.000084606916,0.00010630665,0.0015439587,0.0005704568,0.00036828654,0.0006091778,0.0003094309,0.00032820358],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054902525,0.00014330608,0.8699146,0.00006205352,0.000079952784,0.0028559393,0.0030673745,0.00025848142,0.02579036,0.0037442734,0.002575234,0.09095943],"study_design_scores_gemma":[0.00000360571,0.000044756405,0.9788807,0.000015478658,0.000011254597,0.0028342411,0.0004231081,0.00011807024,0.000642834,0.0006366743,0.016379755,0.000009524055],"about_ca_topic_score_codex":0.023201492,"about_ca_topic_score_gemma":0.026236247,"teacher_disagreement_score":0.023201492,"about_ca_system_score_codex":0.0007959532,"about_ca_system_score_gemma":0.00016819299,"threshold_uncertainty_score":0.046132922},"labels":[],"label_agreement":null},{"id":"W2050437970","doi":"10.1086/522916","title":"Central Relaxation of Dark Matter Halos","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Power law; Dark matter; Adiabatic process; Distribution function; Relaxation (psychology); Logarithm; Statistical physics; Non-equilibrium thermodynamics; Series (stratigraphy); RADIUS; Astrophysics; Quantum mechanics; Mathematical analysis","score_opus":0.005469309333014652,"score_gpt":0.206146102691309,"score_spread":0.20067679335829436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050437970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90039855,0.0004862302,0.08463346,0.0003134891,0.00003193546,0.000017467875,0.00005948353,0.00021784188,0.013841546],"genre_scores_gemma":[0.99480766,0.000111889,0.002369986,0.000022088887,0.000017658725,0.000005659046,0.00002801272,0.000039605664,0.0025974612],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999238,0.000015082831,0.0000026214454,0.000017210059,0.000018749291,0.000022518921],"domain_scores_gemma":[0.9996123,0.000101726306,0.00007472788,0.000057284928,0.00006963512,0.00008448154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040516938,0.00024001753,0.0002145976,0.00044266912,0.00041678525,0.0007624548,0.0005403944,0.00016869232,0.0030233301],"category_scores_gemma":[0.0018662811,0.00014867097,0.00034948008,0.00014868584,0.00081459404,0.0009575977,0.0008343557,0.00046322466,0.00021216657],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033749148,0.00006897818,0.018158164,0.00017010377,0.000049148526,0.000918935,0.0012348476,0.110337116,0.07735729,0.76148295,0.0010864773,0.028798454],"study_design_scores_gemma":[0.00004543448,0.0001425266,0.02446542,0.00002973186,0.000034019093,0.00077613245,0.00038048034,0.69823366,0.026912617,0.24480957,0.00411938,0.00005099648],"about_ca_topic_score_codex":0.0023598177,"about_ca_topic_score_gemma":0.0011146686,"teacher_disagreement_score":0.0030233301,"about_ca_system_score_codex":0.000882505,"about_ca_system_score_gemma":0.0002931257,"threshold_uncertainty_score":0.010114014},"labels":[],"label_agreement":null},{"id":"W2050444070","doi":"10.1088/0004-637x/758/1/63","title":"ON THE MASS RADIATED BY COALESCING BLACK HOLE BINARIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph","funders":"","keywords":"Gravitational wave; Gravitational energy; Black hole (networking); Limit (mathematics); Binary black hole; Waveform; Gravitation; Gravitational-wave observatory; Binary number","score_opus":0.01323803336862936,"score_gpt":0.29103912355699013,"score_spread":0.27780109018836074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050444070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7790986,0.0008950669,0.20500663,0.00028949557,0.000090652706,0.000029165718,0.00013386579,0.00024453038,0.014212069],"genre_scores_gemma":[0.98609316,0.00040272152,0.010720029,0.00004524956,0.00003074396,0.00001910085,0.000058462585,0.000114187584,0.0025161381],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999155,0.000024332492,0.000005157035,0.0000126317445,0.000027819442,0.000014644572],"domain_scores_gemma":[0.99954236,0.00026696586,0.000084648855,0.000040668183,0.000040351817,0.000025052072],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044666842,0.00050956605,0.00034051048,0.00073486834,0.0003238589,0.00041658425,0.0007653638,0.0004757849,0.0030566729],"category_scores_gemma":[0.0028686477,0.0001609781,0.00033225215,0.00046352923,0.00087424985,0.00090319803,0.0008595057,0.00038787027,0.00048541947],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017493518,0.000054865508,0.009007268,0.00019257209,0.00005694809,0.0010240482,0.00029194274,0.72856355,0.027441707,0.2086059,0.00059726555,0.023988988],"study_design_scores_gemma":[0.000017933793,0.000027871236,0.0040146546,0.000020045245,0.000017869941,0.00014028144,0.00004588262,0.9571211,0.005543489,0.03247378,0.0005547331,0.000022467557],"about_ca_topic_score_codex":0.0012842567,"about_ca_topic_score_gemma":0.0010356767,"teacher_disagreement_score":0.0030566729,"about_ca_system_score_codex":0.0005825706,"about_ca_system_score_gemma":0.00016469568,"threshold_uncertainty_score":0.010225594},"labels":[],"label_agreement":null},{"id":"W2050515876","doi":"10.1086/524653","title":"Glitches in Anomalous X‐Ray Pulsars","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Glitch; Pulsar; Physics; Astrophysics; Neutron star; Amplitude; Astronomy; Flux (metallurgy)","score_opus":0.01591475642751888,"score_gpt":0.29653523738058346,"score_spread":0.2806204809530646,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050515876","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953103,0.00012023104,0.000075966,0.0000064662727,0.0000032747453,0.0000022773409,0.000072081995,0.0000067604583,0.00018201846],"genre_scores_gemma":[0.9989096,0.00019221164,0.00016754401,0.0000128677775,0.000023021918,0.0000054697703,0.0005037598,0.0000039661422,0.00018169566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987507,0.000013738509,0.00001568773,0.00003393497,0.000030196961,0.00003138448],"domain_scores_gemma":[0.9993492,0.00007668342,0.00038286464,0.00006193192,0.000048924667,0.00008039327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001904836,0.00024851592,0.00025703755,0.000938822,0.00032117649,0.00037334653,0.000209066,0.00024624716,0.00042977798],"category_scores_gemma":[0.0006833695,0.00013591886,0.0002497025,0.0004486089,0.00033689226,0.00021502176,0.0007897719,0.000277837,0.00015049995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042112658,0.0000614393,0.93441504,0.00004539453,0.000106239924,0.0018743756,0.00032055957,0.00052371074,0.040747937,0.00010693021,0.00018731684,0.02118995],"study_design_scores_gemma":[0.0000040187606,0.0001640391,0.99585706,0.0000031596965,0.000014117278,0.0016728868,0.000044890854,0.00021742118,0.0013772864,0.00004256975,0.000596596,0.000006021746],"about_ca_topic_score_codex":0.00083555037,"about_ca_topic_score_gemma":0.0011598499,"teacher_disagreement_score":0.000938822,"about_ca_system_score_codex":0.00017519997,"about_ca_system_score_gemma":0.00007034625,"threshold_uncertainty_score":0.0016613603},"labels":[],"label_agreement":null},{"id":"W2050637585","doi":"10.1088/0004-637x/697/1/45","title":"ESTIMATING THE PARAMETERS OF SAGITTARIUS A*'s ACCRETION FLOW VIA MILLIMETER VLBI","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Very-long-baseline interferometry; Physics; Millimeter; Supermassive black hole; Accretion (finance); Astrophysics; Sagittarius A*; Parameter space; Black hole (networking); Astronomy; Galaxy; Geometry","score_opus":0.013240251457464174,"score_gpt":0.2354869633128346,"score_spread":0.22224671185537043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050637585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868509,0.0000917079,0.010197841,0.00006599836,0.00000556725,0.000015751662,0.0008224332,0.00023356495,0.0017161975],"genre_scores_gemma":[0.9953798,0.000045972123,0.003107718,0.00002454483,0.000007204704,0.000009903918,0.00128182,0.000018429677,0.00012464655],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99976677,0.00006600244,0.000015989384,0.00006810673,0.00004342305,0.000039767056],"domain_scores_gemma":[0.9993749,0.00011862415,0.00021766115,0.00013244995,0.00007582958,0.00008046315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007399914,0.00042695896,0.000279171,0.000987965,0.0002924075,0.00097321265,0.00045032415,0.0003511245,0.00039137222],"category_scores_gemma":[0.002054954,0.000277667,0.00040768483,0.0006108816,0.00019650465,0.00041596894,0.00047462847,0.0003675382,0.00033306214],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012841652,0.00005242822,0.92041266,0.000023399993,0.00019267418,0.00009854659,0.00011290236,0.037854046,0.016769657,0.0026804402,0.00094610814,0.0207287],"study_design_scores_gemma":[0.000025087314,0.00006543179,0.7796785,0.000016985436,0.000051969986,0.00011713772,0.00013041822,0.2116999,0.0035475043,0.0024704076,0.0021526471,0.00004407389],"about_ca_topic_score_codex":0.009810961,"about_ca_topic_score_gemma":0.0074172923,"teacher_disagreement_score":0.009810961,"about_ca_system_score_codex":0.00066075125,"about_ca_system_score_gemma":0.00037279224,"threshold_uncertainty_score":0.019507706},"labels":[],"label_agreement":null},{"id":"W2050646895","doi":"10.1088/0004-637x/698/1/405","title":"DISCOVERY OF THE WIDEST VERY LOW MASS FIELD BINARY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Sky; Proper motion; Binary number; Stars; Physics; Motion (physics); Astrophysics; Low Mass; Component (thermodynamics); Field (mathematics); Spectral line; Astronomy; Mathematics","score_opus":0.0065441831045667176,"score_gpt":0.20983932627841947,"score_spread":0.20329514317385275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050646895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962788,0.0005449723,0.00045927917,0.00010319319,0.000016566853,0.0000030856017,0.000070963215,0.000015201746,0.002507981],"genre_scores_gemma":[0.9990307,0.000060353537,0.000378246,0.000053518434,0.000015419013,0.0000017318652,0.00013539744,0.000002123689,0.00032249407],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985206,0.000014309239,0.000007923503,0.00005612877,0.000037422644,0.00003221735],"domain_scores_gemma":[0.9995158,0.000085151834,0.00012412414,0.000059082824,0.000063344916,0.00015246753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030134778,0.000106232874,0.0002830094,0.0010010793,0.0009164263,0.0009720145,0.00021508841,0.00048425698,0.0011234905],"category_scores_gemma":[0.0008924425,0.0001634845,0.00008250345,0.00038485005,0.00047599943,0.00036967368,0.0008444384,0.00041097723,0.0004074014],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005600015,0.00019412444,0.7875283,0.00011594619,0.000073395335,0.0034199283,0.0011588483,0.00046181935,0.09130065,0.0054113735,0.0026186763,0.10715692],"study_design_scores_gemma":[0.000040544805,0.0004922833,0.95375454,0.000046705518,0.000060009064,0.016324075,0.00036554044,0.0014651538,0.011373257,0.0026993162,0.013340391,0.00003826519],"about_ca_topic_score_codex":0.0007389569,"about_ca_topic_score_gemma":0.0012533313,"teacher_disagreement_score":0.0011234905,"about_ca_system_score_codex":0.00027001178,"about_ca_system_score_gemma":0.00012760833,"threshold_uncertainty_score":0.0037584305},"labels":[],"label_agreement":null},{"id":"W2050659516","doi":"10.1088/0004-637x/776/2/80","title":"THE PAndAS VIEW OF THE ANDROMEDA SATELLITE SYSTEM. I. A BAYESIAN SEARCH FOR DWARF GALAXIES USING SPATIAL AND COLOR-MAGNITUDE INFORMATION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Andromeda; Dwarf galaxy; Local Group; Milky Way; Dwarf galaxy problem; Galaxy; Globular cluster; Halo","score_opus":0.01145946867497884,"score_gpt":0.2562036833979408,"score_spread":0.24474421472296196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050659516","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.029685952,0.0026701097,0.7691373,0.0020896993,0.00040198764,0.00030658318,0.03527748,0.079285406,0.081145465],"genre_scores_gemma":[0.25281325,0.0012339666,0.6895834,0.0008784384,0.0003813154,0.00025957404,0.02948663,0.004305767,0.021057665],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99962413,0.00007451549,0.000018592365,0.00012620677,0.00012219473,0.000034411525],"domain_scores_gemma":[0.99963415,0.00006379269,0.0000473258,0.0001360179,0.000066517234,0.00005223498],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005434681,0.00077902933,0.0004180679,0.0019144772,0.00047662674,0.0025066289,0.0011588163,0.00063625065,0.012883847],"category_scores_gemma":[0.0013254978,0.000532635,0.00046319704,0.0012275904,0.00053164904,0.001667206,0.0015765325,0.0007731104,0.005724775],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008424348,0.00013760872,0.038953524,0.00070968614,0.0003928,0.000721872,0.00071136595,0.02856066,0.033721168,0.123870485,0.19429617,0.5770823],"study_design_scores_gemma":[0.00012292083,0.000098988516,0.02529393,0.00018253854,0.00009189247,0.0014807263,0.0003818956,0.14684545,0.010518397,0.088893875,0.7259637,0.00012563303],"about_ca_topic_score_codex":0.010042158,"about_ca_topic_score_gemma":0.016878905,"teacher_disagreement_score":0.012883847,"about_ca_system_score_codex":0.00043377184,"about_ca_system_score_gemma":0.00089600356,"threshold_uncertainty_score":0.043100774},"labels":[],"label_agreement":null},{"id":"W2050683067","doi":"10.1086/590552","title":"Outside-In Disk Evolution in the Large Magellanic Cloud","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Large Magellanic Cloud; Star formation; RADIUS; Stellar population; Population; Stellar evolution; Stellar density; Spiral galaxy","score_opus":0.00769796482679193,"score_gpt":0.2112794732202642,"score_spread":0.20358150839347225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050683067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99967563,0.000028034758,0.00004169529,0.0000086204245,3.9483308e-7,5.8741716e-7,0.000032808104,0.0000030862582,0.00020927226],"genre_scores_gemma":[0.99978226,0.000009984761,0.00003376574,0.000002521463,0.00000122731,3.7006862e-7,0.00006029259,0.0000014633777,0.0001082645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993074,0.0000086900445,0.000002227395,0.000019042194,0.000008586346,0.00003066601],"domain_scores_gemma":[0.99944156,0.00008608215,0.00016581143,0.000044853045,0.00007141391,0.00019027735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013253192,0.000123676,0.00015509399,0.0006865518,0.00042308078,0.00060922885,0.00022175611,0.0001888122,0.0008623974],"category_scores_gemma":[0.0006810435,0.0000844408,0.00009158365,0.00044774418,0.0002772411,0.00032120894,0.00029378542,0.00013174693,0.00014285868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002526128,0.00007221827,0.95408994,0.000014523532,0.000023661998,0.0006382117,0.0006739104,0.0018914918,0.032696515,0.0009446425,0.00024621005,0.008456032],"study_design_scores_gemma":[0.000002700432,0.000017172464,0.99707174,0.0000022144998,0.0000054446796,0.00015198597,0.00012718973,0.0013957241,0.0007686809,0.00010965685,0.0003445572,0.0000028418851],"about_ca_topic_score_codex":0.017551491,"about_ca_topic_score_gemma":0.018460188,"teacher_disagreement_score":0.017551491,"about_ca_system_score_codex":0.000981243,"about_ca_system_score_gemma":0.00018799935,"threshold_uncertainty_score":0.03489864},"labels":[],"label_agreement":null},{"id":"W2050753237","doi":"10.1088/0004-637x/729/2/139","title":"THE GEMINI NICI PLANET-FINDING CAMPAIGN: DISCOVERY OF A SUBSTELLAR L DWARF COMPANION TO THE NEARBY YOUNG M DWARF CD–35 2722","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Brown dwarf; Astrometry; Stellar classification; Spectral line; Field (mathematics); Low Mass","score_opus":0.02164696382124804,"score_gpt":0.23028915637575478,"score_spread":0.20864219255450675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050753237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99818474,0.000064578744,0.00009705602,0.000033515476,0.0000032782689,0.000005996325,0.00054563617,0.000033250788,0.0010318513],"genre_scores_gemma":[0.99741995,0.000038428734,0.00035549974,0.000039964896,0.000006411621,0.0000045914617,0.0017385508,0.0000049813566,0.0003915914],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990535,0.000008496065,0.000005107734,0.000031985295,0.00002596119,0.000023041703],"domain_scores_gemma":[0.9997799,0.000021139584,0.000052068757,0.000026245838,0.00002687603,0.00009376739],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017002375,0.00016030014,0.00012126174,0.0006250461,0.0005350651,0.00034914972,0.00025772932,0.00022391387,0.000644671],"category_scores_gemma":[0.0002883666,0.00009263421,0.00008833459,0.00037888973,0.00017875727,0.00011480029,0.00040277332,0.00014204816,0.00023817035],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020699755,0.0000614905,0.9459902,0.00003939744,0.000033175274,0.0014108464,0.0005435842,0.00025957616,0.037665993,0.00020144047,0.0018815446,0.011705672],"study_design_scores_gemma":[0.000007050388,0.000054824995,0.99069935,0.0000051921147,0.00001621154,0.0011769007,0.00021279175,0.00074009015,0.0033346426,0.000032234286,0.0037166015,0.0000039763568],"about_ca_topic_score_codex":0.011293014,"about_ca_topic_score_gemma":0.03049154,"teacher_disagreement_score":0.011293014,"about_ca_system_score_codex":0.000533189,"about_ca_system_score_gemma":0.00024480282,"threshold_uncertainty_score":0.02245456},"labels":[],"label_agreement":null},{"id":"W2050796361","doi":"10.1086/513690","title":"Far‐Infrared<i>Spitzer</i>Observations of Elliptical Galaxies: Evidence for Extended Diffuse Dust","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Dust lane; Galaxy; Interstellar medium; Elliptical galaxy; Cosmic dust; Cooling flow; Flux (metallurgy); Stars; Optical depth","score_opus":0.030872633029319647,"score_gpt":0.268289684688859,"score_spread":0.23741705165953936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050796361","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99593014,0.00018238572,0.00019984652,0.000051456176,0.0000025019651,0.000003822289,0.00019936207,0.000026092443,0.0034043754],"genre_scores_gemma":[0.99897325,0.000096284195,0.00016644002,0.000053257634,0.00001640692,0.0000031341212,0.00023726479,0.0000040530003,0.0004498782],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989796,0.0000036133806,0.0000067552305,0.00003272976,0.000023601897,0.00003524078],"domain_scores_gemma":[0.9992428,0.000065808745,0.00031273882,0.00006319923,0.00011104257,0.00020451786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017555917,0.00017888787,0.00016961247,0.0010116136,0.00020707202,0.000448325,0.000360676,0.00025692632,0.0023493436],"category_scores_gemma":[0.0003294236,0.0001814169,0.00015970346,0.0004780072,0.00063568604,0.0004228901,0.0003793144,0.00017940288,0.00057536416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013508544,0.00005305801,0.9428481,0.000041635307,0.000046374065,0.0004527379,0.00042736586,0.00006546843,0.043651484,0.00026041706,0.0004522102,0.011566115],"study_design_scores_gemma":[0.0000026424532,0.000014345501,0.9988122,0.0000030260303,0.0000045809365,0.00025695795,0.000049041704,0.000030022455,0.00050398544,0.000038972732,0.00028266184,0.000001591584],"about_ca_topic_score_codex":0.002303311,"about_ca_topic_score_gemma":0.0047525265,"teacher_disagreement_score":0.0023493436,"about_ca_system_score_codex":0.00021455178,"about_ca_system_score_gemma":0.00008134601,"threshold_uncertainty_score":0.007859349},"labels":[],"label_agreement":null},{"id":"W2050866319","doi":"10.1088/0004-637x/744/2/159","title":"NEW CONSTRAINTS ON THE EVOLUTION OF THE STELLAR-TO-DARK MATTER CONNECTION: A COMBINED ANALYSIS OF GALAXY-GALAXY LENSING, CLUSTERING, AND STELLAR MASS FUNCTIONS FROM<i>z</i>= 0.2 to<i>z</i>= 1","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":533,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"SLAC National Accelerator Laboratory; Lawrence Berkeley National Laboratory; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; European Southern Observatory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Space Telescope Science Institute; Johns Hopkins University; Centre National d’Etudes Spatiales; Ministry of Education, Culture, Sports, Science and Technology; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Halo; Galaxy; Stellar mass; Redshift; Galaxy formation and evolution; Star formation; Dark matter; Scaling","score_opus":0.0108365565038744,"score_gpt":0.19637477004817813,"score_spread":0.18553821354430372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2050866319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99809235,0.00016147344,0.00095208874,0.000040381525,9.957066e-7,0.0000020317761,0.00021627962,0.00003921182,0.0004951483],"genre_scores_gemma":[0.998718,0.00006085276,0.00059979386,0.000009711152,0.0000049003866,0.0000020636837,0.0005189721,0.0000132657515,0.00007250951],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982303,0.00004278859,0.0000121865505,0.00005392477,0.000029419303,0.000038698687],"domain_scores_gemma":[0.9977963,0.00090198615,0.0006298632,0.00023860401,0.00015293725,0.0002803191],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008860543,0.0004527755,0.0005542067,0.0016739372,0.00042107186,0.0012766338,0.00048358462,0.00055981416,0.00079181214],"category_scores_gemma":[0.003162159,0.00047622912,0.00058301975,0.0013416295,0.0003962096,0.0010951265,0.0013153603,0.00064365,0.00019626028],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001130203,0.00004827164,0.9700665,0.00003876716,0.0002784682,0.00013928382,0.00033715606,0.006563638,0.013998,0.0013153892,0.00020384477,0.0068976996],"study_design_scores_gemma":[0.000010588247,0.00003100908,0.97580045,0.000007078617,0.00007291371,0.000073454816,0.00010776472,0.02126745,0.0013318644,0.00081995316,0.00046276397,0.0000148833],"about_ca_topic_score_codex":0.008291249,"about_ca_topic_score_gemma":0.012748133,"teacher_disagreement_score":0.008291249,"about_ca_system_score_codex":0.00045495754,"about_ca_system_score_gemma":0.0002842498,"threshold_uncertainty_score":0.01648599},"labels":[],"label_agreement":null},{"id":"W2051039108","doi":"10.1088/0004-637x/699/1/603","title":"THE EVOLUTION OF<i>SWIFT</i>/BAT BLAZARS AND THE ORIGIN OF THE MeV BACKGROUND","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":195,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Blazar; Physics; Astrophysics; QSOS; Quasar; Redshift; Active galactic nucleus; Population; Galaxy; Astronomy; Gamma ray","score_opus":0.006650201069829654,"score_gpt":0.2177881389099651,"score_spread":0.21113793784013543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051039108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989631,0.0001032264,0.00007322927,0.000024861503,9.72918e-7,0.0000015446703,0.0003317195,0.00001119248,0.0004901837],"genre_scores_gemma":[0.99863106,0.000040965635,0.00012536178,0.000011029862,0.000003861079,0.000001601462,0.00096983364,0.000010215305,0.00020605446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975246,0.00003112105,0.000015035299,0.00007613682,0.00004829228,0.00007702255],"domain_scores_gemma":[0.9981919,0.00021546715,0.00095050485,0.000113007394,0.00021687047,0.0003121934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004956085,0.00023271014,0.00020796833,0.0011153702,0.00028262867,0.0011076159,0.00031961346,0.000375985,0.0010164551],"category_scores_gemma":[0.001554168,0.00020894264,0.00023872986,0.00082854443,0.00030400956,0.00042183377,0.00037125289,0.00035556502,0.0005162949],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014538276,0.000045817134,0.9888277,0.000005672505,0.00003744128,0.000101401405,0.00012953543,0.0003458934,0.0068881223,0.00024473367,0.0001454342,0.003082826],"study_design_scores_gemma":[0.0000019872186,0.000014290981,0.99913836,0.0000014338453,0.000005325,0.000090298956,0.000032874257,0.00029466624,0.00020842005,0.00003243015,0.0001778683,0.0000021199028],"about_ca_topic_score_codex":0.009055367,"about_ca_topic_score_gemma":0.010378196,"teacher_disagreement_score":0.009055367,"about_ca_system_score_codex":0.00041506445,"about_ca_system_score_gemma":0.0001893482,"threshold_uncertainty_score":0.018005311},"labels":[],"label_agreement":null},{"id":"W2051128239","doi":"10.1086/512029","title":"The Role of Galaxy Interactions and Mergers in Star Formation at<i>z</i> ≤ 1.3: Mid‐Infrared Properties in the<i>Spitzer</i>First Look Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"California Institute of Technology; W. M. Keck Foundation; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Luminosity; Star formation; Luminous infrared galaxy; Astronomy; Redshift; Spitzer Space Telescope; Galaxy formation and evolution; Galaxy merger; Infrared; Telescope","score_opus":0.009344953746256976,"score_gpt":0.20789369575745925,"score_spread":0.19854874201120226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051128239","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99955195,0.00009466165,0.00003726218,0.000019943504,5.102981e-7,0.0000014683087,0.0000875822,0.000004083594,0.00020253561],"genre_scores_gemma":[0.99962854,0.000042285894,0.000055967535,0.000012082515,0.0000030350639,0.0000015658327,0.00019799288,0.0000020935918,0.000056476252],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980694,0.000025426707,0.000012091797,0.000047391757,0.0000453389,0.00006298351],"domain_scores_gemma":[0.99845326,0.00016471035,0.0008129727,0.000057309273,0.000072478535,0.00043925652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041807053,0.0002851575,0.0003221437,0.0015886726,0.0004814675,0.0010916048,0.00038144458,0.0005088739,0.00095985754],"category_scores_gemma":[0.0010895914,0.00032390922,0.00042710427,0.00078798947,0.00051673607,0.0006703754,0.00088360556,0.00034635927,0.00031153907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039949708,0.000010505996,0.9970799,0.000003994424,0.000018470595,0.000030665316,0.0001129584,0.00004364855,0.0018159999,0.0000339238,0.000026716147,0.00078321784],"study_design_scores_gemma":[4.3326168e-7,0.0000071861155,0.9998,7.303852e-7,0.0000044413964,0.000029535768,0.000033389188,0.000047413396,0.000049477916,0.0000061557207,0.000020482139,7.174506e-7],"about_ca_topic_score_codex":0.0070892856,"about_ca_topic_score_gemma":0.011904882,"teacher_disagreement_score":0.0070892856,"about_ca_system_score_codex":0.0003622163,"about_ca_system_score_gemma":0.00017207173,"threshold_uncertainty_score":0.014096022},"labels":[],"label_agreement":null},{"id":"W2051139634","doi":"10.1088/0004-637x/793/2/79","title":"HZ HER: STELLAR RADIUS FROM X-RAY ECLIPSE OBSERVATIONS, EVOLUTIONARY STATE, AND A NEW DISTANCE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; RADIUS; Neutron star; Metallicity; Eclipse; Orbital inclination; Effective temperature; Stellar mass; Star (game theory); Mass ratio; Star formation; Galaxy; Stars; Binary number","score_opus":0.015927719570182873,"score_gpt":0.2146183898672043,"score_spread":0.19869067029702142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051139634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98795426,0.00022197531,0.0016191322,0.00005689142,0.000012217692,0.000010911148,0.0046937666,0.0002594063,0.0051714047],"genre_scores_gemma":[0.9893197,0.00007371965,0.0018272633,0.000013570795,0.000011599505,0.0000070813835,0.0074351504,0.00006247342,0.0012494285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982625,0.00001830649,0.000009179536,0.000070452894,0.000052370724,0.000023569568],"domain_scores_gemma":[0.99961734,0.000053526368,0.00011831438,0.000072609975,0.00007051358,0.00006758441],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037512934,0.00024314011,0.00018812701,0.0005730396,0.0001356714,0.00040784598,0.00033881498,0.0002789688,0.0021075006],"category_scores_gemma":[0.00082256703,0.00011971839,0.0002279735,0.00035800345,0.00014388331,0.00047859072,0.00052054605,0.00020008672,0.0009799639],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021846048,0.000028960707,0.9610627,0.00008693596,0.00010620111,0.00012783597,0.00016885794,0.010681895,0.007632128,0.0012145197,0.0032520639,0.015419352],"study_design_scores_gemma":[0.000010525248,0.000034878627,0.976149,0.000010989395,0.000031215306,0.00028381296,0.00007830377,0.014813827,0.0025775037,0.00029245962,0.0057005878,0.000016906848],"about_ca_topic_score_codex":0.005602426,"about_ca_topic_score_gemma":0.012095172,"teacher_disagreement_score":0.005602426,"about_ca_system_score_codex":0.00048018576,"about_ca_system_score_gemma":0.00015945986,"threshold_uncertainty_score":0.011139631},"labels":[],"label_agreement":null},{"id":"W2051140708","doi":"10.1088/0004-637x/776/2/65","title":"REGIONAL VARIATIONS IN THE DENSE GAS HEATING AND COOLING IN M51 FROM<i>HERSCHEL</i>FAR-INFRARED SPECTROSCOPY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Jet Propulsion Laboratory; Centre National d’Etudes Spatiales; Bundesministerium für Verkehr, Innovation und Technologie; Centre National de la Recherche Scientifique; KU Leuven; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; California Institute of Technology; Imperial College London; UK Space Agency; Max-Planck-Institut für Astronomie; Cardiff University","keywords":"Flux (metallurgy); Spectroscopy; Spire (mollusc); Radiation; Radiation flux; Photon; Falling (accident); Radiative cooling","score_opus":0.008962858788449764,"score_gpt":0.21692457406495363,"score_spread":0.20796171527650387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051140708","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998221,0.00015352957,0.00008010303,0.00002304887,0.0000015193087,0.0000017770363,0.0004079559,0.00002002574,0.0010911084],"genre_scores_gemma":[0.99906534,0.00004123046,0.00012556683,0.0000119663755,0.0000036357678,0.0000017769661,0.00058287074,0.0000048328475,0.00016281978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987674,0.00001079637,0.0000053783006,0.00004739389,0.000029534145,0.000030165005],"domain_scores_gemma":[0.99969065,0.000041965068,0.00014149428,0.00005124867,0.00004032402,0.00003438049],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019887873,0.00020345316,0.00015992137,0.0008727638,0.00025830595,0.00043221473,0.0002310923,0.00029701256,0.0009573522],"category_scores_gemma":[0.0005379687,0.00015579477,0.00021302217,0.00048913225,0.0002535912,0.00027438402,0.00045577553,0.00012949752,0.00039205226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021790073,0.000028080356,0.9202044,0.00004665165,0.00014691982,0.00025384309,0.0005647782,0.0020390863,0.061661944,0.0003637469,0.0010977734,0.013374804],"study_design_scores_gemma":[0.0000011498603,0.0000043637638,0.99915826,0.0000015724014,0.0000050573112,0.000029697232,0.000017581642,0.00018108435,0.00037266887,0.0000073342867,0.00021958734,0.0000015827885],"about_ca_topic_score_codex":0.009911953,"about_ca_topic_score_gemma":0.01992397,"teacher_disagreement_score":0.009911953,"about_ca_system_score_codex":0.00049075164,"about_ca_system_score_gemma":0.0000775543,"threshold_uncertainty_score":0.019708514},"labels":[],"label_agreement":null},{"id":"W2051169733","doi":"10.1086/322320","title":"Transport of Magnetic Fields in Convective, Accreting Supernova Cores","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Neutron star; Supernova; Magnetic field; Pulsar; Convection; Hydrostatic equilibrium; Opacity; Neutrino; Magnetohydrodynamics","score_opus":0.012411199171301748,"score_gpt":0.2979420016949923,"score_spread":0.28553080252369056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051169733","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99090517,0.00032203848,0.0043313447,0.00007511984,0.000016341834,0.000019703726,0.00008828282,0.000048073114,0.00419393],"genre_scores_gemma":[0.99788684,0.00018618067,0.0009003611,0.000012737234,0.00001024651,0.000010294387,0.000044030185,0.00001334423,0.0009359172],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995494,0.000009302873,0.0000026610305,0.0000064938204,0.000009189741,0.000017408736],"domain_scores_gemma":[0.99982196,0.00006300002,0.000048321486,0.000009569392,0.00002298772,0.00003422607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001837073,0.00031793135,0.00022561029,0.0005621133,0.0005157325,0.0008170678,0.00048214765,0.00048276206,0.00053549005],"category_scores_gemma":[0.0010112595,0.00021688997,0.00032320377,0.0003728237,0.00078084355,0.00044259866,0.0006247263,0.00025615684,0.00008620716],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002769107,0.00009431813,0.020242512,0.000062218714,0.00006053504,0.00052341673,0.00016162626,0.94251966,0.019471304,0.012080161,0.00019838779,0.004308945],"study_design_scores_gemma":[0.00005006093,0.000102484606,0.009043124,0.000012352216,0.000019480209,0.0000702176,0.00008083437,0.9847705,0.0027220487,0.0025339627,0.0005779174,0.000017014192],"about_ca_topic_score_codex":0.013037384,"about_ca_topic_score_gemma":0.0047561997,"teacher_disagreement_score":0.013037384,"about_ca_system_score_codex":0.0011471518,"about_ca_system_score_gemma":0.00048162794,"threshold_uncertainty_score":0.025923014},"labels":[],"label_agreement":null},{"id":"W2051365623","doi":"10.1086/345788","title":"The Structural Evolution of Substructure","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":400,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; University of Victoria","funders":"","keywords":"Substructure; Halo; Dark matter; Milky Way; Galaxy; RADIUS; Dwarf galaxy problem; Dark matter halo; Cold dark matter","score_opus":0.006307975094039132,"score_gpt":0.24902582725229416,"score_spread":0.24271785215825503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051365623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958372,0.000092219045,0.0015389951,0.0001069419,0.0000067439655,0.0000141101855,0.00015234918,0.00004688362,0.0022046631],"genre_scores_gemma":[0.9987,0.00006793973,0.00066489854,0.000025284147,0.0000037539905,0.000008205852,0.00013915647,0.000021184223,0.00036946507],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999008,0.000021332035,0.0000044978515,0.00001797513,0.00001695205,0.00003837698],"domain_scores_gemma":[0.9994017,0.000121048506,0.0001168071,0.00007550039,0.00007154085,0.0002135414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039835586,0.00041122726,0.00036142033,0.0005976762,0.0009026328,0.001229995,0.0009856485,0.0007450504,0.0016798682],"category_scores_gemma":[0.0018361195,0.00035597442,0.00068644877,0.0005225729,0.0009337016,0.000722835,0.0010677705,0.00055797474,0.00022137482],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012143406,0.00008416089,0.0654628,0.000031193184,0.0001433524,0.0003338798,0.00027470154,0.92193395,0.005921789,0.0031030648,0.00027695746,0.0023126872],"study_design_scores_gemma":[0.00005613077,0.00009922076,0.02623393,0.000010873583,0.00003545073,0.00007392478,0.00015114433,0.96989274,0.0008109167,0.0020884955,0.0005244585,0.000022793476],"about_ca_topic_score_codex":0.029261686,"about_ca_topic_score_gemma":0.015596408,"teacher_disagreement_score":0.029261686,"about_ca_system_score_codex":0.001324408,"about_ca_system_score_gemma":0.00071833946,"threshold_uncertainty_score":0.058182716},"labels":[],"label_agreement":null},{"id":"W2051374903","doi":"10.1088/0004-637x/792/2/110","title":"THREE ANCIENT HALO SUBGIANTS: PRECISE PARALLAXES, COMPOSITIONS, AGES, AND IMPLICATIONS FOR GLOBULAR CLUSTERS, ,","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Globular cluster; RR Lyrae variable; Population; Stars; Halo; Stellar population; Horizontal branch; Age of the universe; Apparent magnitude","score_opus":0.013186434075513627,"score_gpt":0.23877037874663243,"score_spread":0.2255839446711188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051374903","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9813208,0.005126202,0.009323244,0.0002742511,0.000020965816,0.000006680295,0.00063381577,0.000078632955,0.0032154254],"genre_scores_gemma":[0.99502003,0.00076002773,0.0031927568,0.000039153798,0.000012205098,0.0000035326977,0.00027875538,0.000014743628,0.00067872804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999871,0.00002301008,0.000010676808,0.0000493046,0.00003056561,0.00001539344],"domain_scores_gemma":[0.99952984,0.00010661521,0.00013212023,0.00009548818,0.00008069142,0.000055266268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000817232,0.0002449562,0.00016694177,0.00060137094,0.00037331966,0.00092414464,0.00037934026,0.00030989587,0.00070057187],"category_scores_gemma":[0.0014759985,0.00015388956,0.000095598516,0.000718725,0.00048418375,0.0007179063,0.0006478158,0.0004363475,0.00028499332],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024332042,0.000021275402,0.8727959,0.00014808857,0.00006170101,0.00021637489,0.0008776879,0.0044704294,0.04568929,0.006328655,0.0004264066,0.06872087],"study_design_scores_gemma":[0.00000745795,0.000029593266,0.9838663,0.000021843402,0.000026888425,0.00015038322,0.00021151865,0.0022144949,0.0074505606,0.0025886623,0.0034172202,0.000015149224],"about_ca_topic_score_codex":0.0034940685,"about_ca_topic_score_gemma":0.008084624,"teacher_disagreement_score":0.0034940685,"about_ca_system_score_codex":0.00045661005,"about_ca_system_score_gemma":0.00025596397,"threshold_uncertainty_score":0.006947458},"labels":[],"label_agreement":null},{"id":"W2051431923","doi":"10.1088/0004-637x/725/2/1485","title":"THE FORMATION OF LOW-MASS BINARY STAR SYSTEMS VIA TURBULENT FRAGMENTATION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":270,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Dimensionless quantity; Radiative transfer; Star formation; Turbulence; Astrophysics; Fragmentation (computing); Binary number; Stars; Instability; Circumstellar disk; Gravitation; Mechanics; Classical mechanics; Optics","score_opus":0.006146425076232871,"score_gpt":0.22547631832811602,"score_spread":0.21932989325188315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051431923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991059,0.000026161295,0.00052788306,0.000017851753,8.095102e-7,0.0000033347317,0.00001631549,0.00001639488,0.00028542816],"genre_scores_gemma":[0.99968207,0.000011723304,0.00023483667,0.0000035455591,7.767227e-7,0.000001826499,0.00002296774,0.0000031488364,0.000039121533],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998988,0.000027548316,0.0000064036817,0.000015514872,0.000018085813,0.0000335729],"domain_scores_gemma":[0.99875844,0.00052336504,0.0003487219,0.00008506979,0.000069220834,0.00021526711],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003134628,0.00040020992,0.00025704099,0.0003325564,0.000433579,0.0006148938,0.0003765099,0.0003229084,0.0004812821],"category_scores_gemma":[0.0027434116,0.00015843229,0.00025302632,0.00025661933,0.00068288966,0.00058921246,0.00046211435,0.00029984151,0.000062809784],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005950636,0.00027020375,0.2713032,0.00009813299,0.00018177005,0.00080215547,0.00075256283,0.646563,0.06063243,0.011042294,0.00040657967,0.007352678],"study_design_scores_gemma":[0.00006121844,0.0001856474,0.039312817,0.000007103227,0.000036921992,0.00023715875,0.00014871905,0.946698,0.00989578,0.0031396283,0.0002533289,0.000023681014],"about_ca_topic_score_codex":0.0030227953,"about_ca_topic_score_gemma":0.0020109056,"teacher_disagreement_score":0.0030227953,"about_ca_system_score_codex":0.000750142,"about_ca_system_score_gemma":0.0002725267,"threshold_uncertainty_score":0.006010413},"labels":[],"label_agreement":null},{"id":"W2051438108","doi":"10.1086/319781","title":"The Nuclear Dynamics of M32. I. Data and Stellar Kinematics","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Kinematics; Dynamics (music); Astronomy; Physics; Astrophysics; Classical mechanics","score_opus":0.01788202173003215,"score_gpt":0.24183439393112074,"score_spread":0.2239523722010886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051438108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982767,0.000095481395,0.00025484033,0.000023534927,0.0000011867324,0.0000053641206,0.00060233125,0.000026664955,0.00071385666],"genre_scores_gemma":[0.9954045,0.00007225668,0.0012605423,0.000009969865,0.000004221748,0.000010923159,0.002844063,0.000018277467,0.0003751572],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986315,0.000019257346,0.000009706093,0.000038494552,0.000041641633,0.000027818942],"domain_scores_gemma":[0.99916553,0.000081210186,0.00027812488,0.00016010409,0.000177142,0.00013791781],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003852399,0.00031217324,0.00023345281,0.00066404085,0.0004867472,0.0003634078,0.0003395364,0.00024185228,0.000885853],"category_scores_gemma":[0.00117825,0.0001691591,0.00018059554,0.00083132496,0.00032427104,0.00034293756,0.0006089505,0.00022057419,0.0006910639],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067971327,0.00007934722,0.8899428,0.00009648102,0.000030213643,0.00057282427,0.0012810787,0.0038868282,0.0814081,0.0009320953,0.0006293599,0.020461226],"study_design_scores_gemma":[0.00002801552,0.00021490462,0.9804741,0.000022746504,0.000016256581,0.0006562764,0.0003191938,0.0046066963,0.0074632294,0.0007134838,0.0054649194,0.000020108648],"about_ca_topic_score_codex":0.006955023,"about_ca_topic_score_gemma":0.010653225,"teacher_disagreement_score":0.006955023,"about_ca_system_score_codex":0.0005309636,"about_ca_system_score_gemma":0.00024295332,"threshold_uncertainty_score":0.013829112},"labels":[],"label_agreement":null},{"id":"W2051763709","doi":"10.1088/0004-637x/791/2/98","title":"SEARCHING FOR DUST AROUND HYPER METAL POOR STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Stars; Circumstellar dust; Flux (metallurgy); RADIUS; Cosmic dust; Debris; Spectral line; Debris disk","score_opus":0.016855240645333662,"score_gpt":0.2602378176306827,"score_spread":0.24338257698534904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051763709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9884163,0.000762349,0.0005581359,0.00046293298,0.000027470158,0.000016826478,0.00038606176,0.00006636368,0.009303557],"genre_scores_gemma":[0.9954862,0.00029637807,0.0008514165,0.00011026689,0.00003187258,0.000006562793,0.0003693031,0.000015635216,0.002832262],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998957,0.000012526132,0.0000052143787,0.000033082066,0.000030393529,0.000022991957],"domain_scores_gemma":[0.9995789,0.00006873981,0.0001121285,0.000025337018,0.00008981588,0.00012504199],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014411165,0.000102095975,0.00020679481,0.0011883401,0.0010774645,0.0009578992,0.00029724176,0.00035827694,0.0033431407],"category_scores_gemma":[0.000919746,0.000107634005,0.00011593858,0.0009589786,0.0003334574,0.00059538835,0.00075091585,0.00020198473,0.0007693476],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020205736,0.000075371456,0.91151047,0.000114970164,0.000056540255,0.0007732196,0.0023967335,0.00051263,0.0157951,0.0009688774,0.0048673563,0.0627267],"study_design_scores_gemma":[0.000011537015,0.000039484912,0.9754474,0.00004608455,0.000025329868,0.00031208864,0.005022451,0.0010229197,0.0017189841,0.0012249146,0.01511902,0.0000096444655],"about_ca_topic_score_codex":0.010185366,"about_ca_topic_score_gemma":0.021229485,"teacher_disagreement_score":0.010185366,"about_ca_system_score_codex":0.0003700831,"about_ca_system_score_gemma":0.00034684778,"threshold_uncertainty_score":0.020252168},"labels":[],"label_agreement":null},{"id":"W2051805217","doi":"10.1086/424962","title":"H<scp>i</scp>Distribution and Kinematics of UGCA 86","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Penticton Regional Hospital; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Calgary","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Astronomy; Thick disk; Galaxy","score_opus":0.006076140633936265,"score_gpt":0.2072016232114213,"score_spread":0.20112548257748503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051805217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8201087,0.00051728706,0.0005713583,0.0010821542,0.00010684181,0.000057915804,0.066684306,0.0010178611,0.109853595],"genre_scores_gemma":[0.9305918,0.00015731143,0.000563385,0.0003416233,0.00009998502,0.000027395296,0.03442669,0.00024998916,0.033541862],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997454,0.000029894265,0.000008219262,0.000048132715,0.00006888706,0.00009943216],"domain_scores_gemma":[0.99848,0.00014183708,0.00027104974,0.000188611,0.0003281119,0.00059036654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002885022,0.00018884659,0.0002645749,0.0020426374,0.00052088156,0.0008918832,0.00034076947,0.00037255723,0.014055722],"category_scores_gemma":[0.0011783475,0.00017696994,0.00029824977,0.002138424,0.00027997437,0.00022376598,0.00047374706,0.00034165103,0.0070699253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009714475,0.0002233918,0.6789813,0.00016437717,0.0001831713,0.0003416378,0.0006448952,0.003226931,0.0074051605,0.0091526015,0.24071331,0.057991885],"study_design_scores_gemma":[0.000011191261,0.00002564832,0.9869294,0.0000073187407,0.000010406444,0.000051511874,0.00004800936,0.00046238425,0.0003513701,0.00017667189,0.01191701,0.000009046251],"about_ca_topic_score_codex":0.04164009,"about_ca_topic_score_gemma":0.034024946,"teacher_disagreement_score":0.04164009,"about_ca_system_score_codex":0.0008298632,"about_ca_system_score_gemma":0.00051740336,"threshold_uncertainty_score":0.08279544},"labels":[],"label_agreement":null},{"id":"W2051907193","doi":"10.1086/521810","title":"<i>Hubble Space Telescope</i>and<i>Spitzer</i>Imaging of Red and Blue Galaxies at<i>z</i>∼ 2.5: A Correlation between Size and Star Formation Activity from Compact Quiescent Galaxies to Extended Star‐forming Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":252,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Elliptical galaxy; Surface brightness; Star formation; Redshift; Stellar mass; Luminous infrared galaxy","score_opus":0.008185484840834643,"score_gpt":0.22209514694098756,"score_spread":0.21390966210015291,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051907193","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982046,0.0000743842,0.000116233634,0.000023457647,0.0000015907448,0.0000032819785,0.0005240332,0.00003313783,0.0010192794],"genre_scores_gemma":[0.99845815,0.000060553815,0.00023530553,0.000025413967,0.00001315332,0.00000424365,0.00091622694,0.0000062927375,0.0002804911],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998988,0.0000060018574,0.000007939394,0.000028189128,0.00002458423,0.00003444768],"domain_scores_gemma":[0.999539,0.00004414403,0.0002206909,0.00003489923,0.000038807866,0.00012249175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001776567,0.00020639058,0.00014875364,0.0015720723,0.00018663016,0.0005207011,0.0002396544,0.00023389708,0.0017946261],"category_scores_gemma":[0.00035291218,0.0001938949,0.00020933368,0.0006752843,0.00024696148,0.00035275982,0.00029462998,0.00017501345,0.00032286163],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014687795,0.000062402585,0.9695125,0.000022745353,0.000043273678,0.00013164547,0.0002187006,0.00036913314,0.02377919,0.00015677106,0.00073247706,0.004824297],"study_design_scores_gemma":[0.0000020973487,0.000007897765,0.9991642,0.0000013922247,0.0000064669644,0.000072853334,0.000023215876,0.0001327709,0.00043885072,0.000013745143,0.00013504436,0.0000014440224],"about_ca_topic_score_codex":0.0058908733,"about_ca_topic_score_gemma":0.012432476,"teacher_disagreement_score":0.0058908733,"about_ca_system_score_codex":0.00027979558,"about_ca_system_score_gemma":0.00010222749,"threshold_uncertainty_score":0.011713147},"labels":[],"label_agreement":null},{"id":"W2051918640","doi":"10.1086/502964","title":"Asteroseismological Studies of Long‐Period Variable Subdwarf B Stars. I. A Multisite Campaign on PG 1627+017","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Subdwarf; Astrophysics; Photometry (optics); Amplitude; Asteroseismology; Stars; Rotation period; Brightness; Differential rotation; Variable star; Astronomy; White dwarf","score_opus":0.017770893619590777,"score_gpt":0.24734433962270264,"score_spread":0.22957344600311186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051918640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992594,0.000039391292,0.00024372888,0.000008882092,0.0000013431313,0.0000052929818,0.0001703148,0.000011688602,0.00025988414],"genre_scores_gemma":[0.997948,0.00004468205,0.0006041818,0.000006176448,0.0000060293387,0.000008170323,0.0011983078,0.000007682998,0.00017681904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.000031973188,0.0000065530903,0.00003529496,0.00002600359,0.000022397606],"domain_scores_gemma":[0.9995009,0.00011226741,0.000092473965,0.00008893033,0.000053528096,0.00015196444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041461087,0.00027851117,0.00032115105,0.0009587913,0.00047292406,0.00028087324,0.00027768605,0.00030042182,0.00051586475],"category_scores_gemma":[0.0004983558,0.00016649744,0.0003851881,0.0005695077,0.00022058637,0.00020348963,0.00045680575,0.0002633814,0.00023202132],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035940215,0.00013906969,0.940843,0.0000656786,0.00013272362,0.00086545816,0.0007565759,0.009534273,0.028994603,0.00034092102,0.00031487085,0.01765345],"study_design_scores_gemma":[0.00001800255,0.00015147925,0.9887949,0.000005453183,0.000023700493,0.00017376692,0.00014606527,0.0076800594,0.0018737275,0.00012677042,0.000997664,0.000008327863],"about_ca_topic_score_codex":0.004367486,"about_ca_topic_score_gemma":0.0074203606,"teacher_disagreement_score":0.004367486,"about_ca_system_score_codex":0.00041315873,"about_ca_system_score_gemma":0.0001805499,"threshold_uncertainty_score":0.008684158},"labels":[],"label_agreement":null},{"id":"W2051935336","doi":"10.1086/318234","title":"Gravity Modes in ZZ Ceti Stars. IV. Amplitude Saturation by Parametric Instability","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Instability; Amplitude; Parametric statistics; Nonlinear system; Parametric oscillator; Excited state; Envelope (radar); Maxima; Stars","score_opus":0.01396937929042421,"score_gpt":0.24082633618749405,"score_spread":0.22685695689706983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051935336","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99662775,0.00013622582,0.0007434734,0.000031523698,0.0000022946763,0.0000051207912,0.00006824402,0.000017616552,0.0023677943],"genre_scores_gemma":[0.9994892,0.000030997115,0.00018437493,0.000005794014,0.0000016824471,0.0000025458933,0.0000598797,0.0000045351017,0.00022103394],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999312,0.0000042631773,0.0000069914327,0.00002472389,0.00001713196,0.000015641044],"domain_scores_gemma":[0.999795,0.000029464583,0.000081416416,0.000021080274,0.00002836477,0.000044710647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011541848,0.00022935336,0.00016823677,0.0006686829,0.00034686466,0.00053995085,0.00021294561,0.00030937692,0.0007571641],"category_scores_gemma":[0.00047189262,0.0001996052,0.00024025864,0.00042946162,0.0003746954,0.00031111788,0.0007614009,0.00029207315,0.00021257011],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004961677,0.00005383939,0.49593502,0.00012397068,0.0000499765,0.0005342558,0.0008899522,0.009331483,0.45991606,0.0057852557,0.00033926667,0.026544688],"study_design_scores_gemma":[0.00006398126,0.00026948858,0.8771706,0.000025957908,0.000038036742,0.00096829777,0.0005715922,0.067183994,0.04524578,0.006419175,0.00199938,0.000043616077],"about_ca_topic_score_codex":0.0015308755,"about_ca_topic_score_gemma":0.0012802297,"teacher_disagreement_score":0.0015308755,"about_ca_system_score_codex":0.00042692432,"about_ca_system_score_gemma":0.000082831706,"threshold_uncertainty_score":0.0030975342},"labels":[],"label_agreement":null},{"id":"W2051953400","doi":"10.1088/0004-637x/717/2/603","title":"THE ACS FORNAX CLUSTER SURVEY. VIII. THE LUMINOSITY FUNCTION OF GLOBULAR CLUSTERS IN VIRGO AND FORNAX EARLY-TYPE GALAXIES AND ITS USE AS A DISTANCE INDICATOR","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":164,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Virgo Cluster; Fornax Cluster; Galaxy; Luminosity function; Luminosity; Galaxy cluster","score_opus":0.0077040968575418705,"score_gpt":0.2090359195867402,"score_spread":0.20133182272919833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2051953400","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.43537384,0.0020104095,0.001746929,0.0006985671,0.00017504202,0.00034324013,0.5221504,0.0019327285,0.0355688],"genre_scores_gemma":[0.4280499,0.0010177718,0.0072528063,0.00019425162,0.00022591637,0.00037642478,0.5384501,0.00029689746,0.024135947],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996736,0.00004177493,0.000021998372,0.00009224155,0.00011387215,0.00005639333],"domain_scores_gemma":[0.99923587,0.00004497135,0.00021341456,0.00014213547,0.0002087177,0.00015485662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005387145,0.00042451944,0.00044707803,0.0043577477,0.0003175318,0.0006038809,0.0007668801,0.00042654137,0.008592186],"category_scores_gemma":[0.0010104332,0.00011445957,0.00032550565,0.0025971492,0.00010121348,0.00036931824,0.0007755303,0.00027664384,0.005843694],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008448371,0.00025066646,0.60392106,0.0006578547,0.00057811575,0.00034430303,0.0005562217,0.0015564159,0.008716792,0.0033366352,0.2548081,0.12442902],"study_design_scores_gemma":[0.00005800455,0.000044368444,0.92224056,0.00003350214,0.00004781455,0.00009765112,0.000110773384,0.0006414163,0.0006958412,0.00033623053,0.075681046,0.000012687586],"about_ca_topic_score_codex":0.03222101,"about_ca_topic_score_gemma":0.023593608,"teacher_disagreement_score":0.03222101,"about_ca_system_score_codex":0.00082432857,"about_ca_system_score_gemma":0.00051023526,"threshold_uncertainty_score":0.06406695},"labels":[],"label_agreement":null},{"id":"W2052024199","doi":"10.1088/0004-637x/802/1/64","title":"CROSS-CORRELATION BETWEEN THE CMB LENSING POTENTIAL MEASURED BY<i>PLANCK</i>AND HIGH-<i>z</i>SUBMILLIMETER GALAXIES DETECTED BY THE<i>HERSCHEL</i>-ATLAS SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Cosmic microwave background; Astrophysics; Galaxy; Planck; Redshift; Atlas (anatomy); Spectral density; Sky; Sigma; Amplitude; Astronomy; Statistics; Optics; Anisotropy","score_opus":0.014606248432716476,"score_gpt":0.22080444528682852,"score_spread":0.20619819685411206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052024199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973328,0.00009173298,0.0006453074,0.000026178579,0.0000033917115,0.0000029703633,0.000713146,0.000039684848,0.0011446443],"genre_scores_gemma":[0.9987644,0.000030124522,0.00030557255,0.000006418929,0.000011221416,0.0000028498334,0.0007774894,0.0000056480058,0.00009628049],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958247,0.00008612944,0.000023221255,0.00012040614,0.00011587597,0.00007199213],"domain_scores_gemma":[0.9947024,0.0019237713,0.0021372424,0.00038722975,0.00041730754,0.00043207666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007569946,0.00035130393,0.00022299627,0.0017928556,0.00016372318,0.00055972696,0.00033842,0.00027959986,0.0020057228],"category_scores_gemma":[0.0036119197,0.00021067105,0.00020932431,0.0013953574,0.00036910054,0.00037949398,0.00069255393,0.00030610617,0.00040199806],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006646379,0.000015712336,0.99247485,0.000016667433,0.00012016448,0.00005898601,0.000064347136,0.0003919758,0.0034107147,0.0002264568,0.00018317845,0.002970386],"study_design_scores_gemma":[0.0000015733101,0.000017252845,0.9975642,0.0000017829299,0.000021716163,0.0000646567,0.000019649551,0.0009991312,0.0010862099,0.000072258365,0.0001458343,0.0000058384967],"about_ca_topic_score_codex":0.001678913,"about_ca_topic_score_gemma":0.0027519176,"teacher_disagreement_score":0.0020057228,"about_ca_system_score_codex":0.0003172153,"about_ca_system_score_gemma":0.00010824179,"threshold_uncertainty_score":0.006709814},"labels":[],"label_agreement":null},{"id":"W2052053901","doi":"10.1086/374806","title":"A New Search Technique for Short Orbital Period Binary Pulsars","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Orbital period; Astrophysics; Sideband; Binary pulsar; Harmonics; Binary number; Orbital elements; Orbital motion; X-ray pulsar; Amplitude; Fourier analysis; Fourier transform; Astronomy; Millisecond pulsar; Optics; Angular momentum; Classical mechanics","score_opus":0.017867214656695003,"score_gpt":0.3336277887411599,"score_spread":0.3157605740844649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052053901","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.05964191,0.0013712518,0.9270267,0.0003269304,0.00020565941,0.00012187649,0.00031813962,0.0021888148,0.008798705],"genre_scores_gemma":[0.13922861,0.00055191433,0.85158944,0.00027019094,0.00018313724,0.00018556055,0.00050505187,0.0002599948,0.007226097],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996252,0.000037825223,0.000023324832,0.00009747121,0.00017690942,0.00003912777],"domain_scores_gemma":[0.9993444,0.00018833802,0.00009224098,0.00016883011,0.00015119999,0.00005504532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003469834,0.0003157143,0.00067039265,0.0013587847,0.0005416979,0.00066390896,0.0007167862,0.00060973805,0.004222026],"category_scores_gemma":[0.0010503302,0.0002970307,0.00040457,0.0012351272,0.00031880944,0.001615319,0.0010840895,0.00067442475,0.0019813257],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025140823,0.00009732192,0.0048715454,0.00020136916,0.00006782292,0.0004231434,0.00020605585,0.0011518138,0.36702013,0.009508918,0.0041196593,0.6120809],"study_design_scores_gemma":[0.0003997931,0.0014581891,0.037924632,0.00013124378,0.00046609546,0.023278631,0.00036669447,0.18094888,0.4733206,0.049726985,0.23164028,0.00033807877],"about_ca_topic_score_codex":0.00024037206,"about_ca_topic_score_gemma":0.0005205386,"teacher_disagreement_score":0.004222026,"about_ca_system_score_codex":0.00010542676,"about_ca_system_score_gemma":0.00034923977,"threshold_uncertainty_score":0.014124095},"labels":[],"label_agreement":null},{"id":"W2052111611","doi":"10.1088/0004-637x/703/1/348","title":"A BRIGHT SUBMILLIMETER SOURCE IN THE BULLET CLUSTER (1E0657-56) FIELD DETECTED WITH BLAST","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy; Telescope; Astronomy; Infrared; Millimeter; Redshift; Gravitational lens; Luminosity; Far infrared; Photometry (optics); Cluster (spacecraft); Virgo Cluster; Galaxy cluster","score_opus":0.0040698059808198335,"score_gpt":0.18662448168675785,"score_spread":0.18255467570593803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052111611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99692684,0.00009470098,0.00027669704,0.00004515611,0.000015020912,0.000012673242,0.00044479995,0.00003954043,0.002144588],"genre_scores_gemma":[0.9954526,0.00007943579,0.001541556,0.0000539921,0.00003483991,0.000008559851,0.001271246,0.000007183454,0.0015506475],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999143,0.0000044335025,0.0000033990445,0.000026977566,0.000028862962,0.000021989385],"domain_scores_gemma":[0.9997986,0.000026666516,0.00006043064,0.000017656917,0.000016449612,0.00008018879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015447573,0.00020855175,0.0003524927,0.00073290203,0.0004988931,0.00032539517,0.00034292744,0.00038305015,0.0023995326],"category_scores_gemma":[0.00022778187,0.00018492452,0.00015208914,0.0005290302,0.0002582668,0.00015599649,0.00063562,0.00025919976,0.0007781701],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011198843,0.00043399842,0.6667885,0.0002059425,0.0001040316,0.008644578,0.0009786757,0.0010609361,0.26154897,0.0016399005,0.0050941007,0.052380394],"study_design_scores_gemma":[0.00002522533,0.00014004418,0.9919945,0.0000111142435,0.00002012827,0.0017316419,0.00009446945,0.0005742693,0.0035139613,0.000096988384,0.0017895806,0.000008104899],"about_ca_topic_score_codex":0.0039358577,"about_ca_topic_score_gemma":0.009302222,"teacher_disagreement_score":0.0039358577,"about_ca_system_score_codex":0.00029246605,"about_ca_system_score_gemma":0.00015570773,"threshold_uncertainty_score":0.008027256},"labels":[],"label_agreement":null},{"id":"W2052267529","doi":"10.1088/0004-637x/755/2/111","title":"A NEW MONTE CARLO METHOD FOR TIME-DEPENDENT NEUTRINO RADIATION TRANSPORT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Monte Carlo method; Physics; Neutrino; Monte Carlo method for photon transport; Statistical physics; Monte Carlo molecular modeling; Dynamic Monte Carlo method; Quantum Monte Carlo; Diffusion Monte Carlo; Hybrid Monte Carlo; Supernova; Kinetic Monte Carlo; Photon; Monte Carlo method in statistical physics; Type II supernova; Photon transport in biological tissue; Computational physics; Markov chain Monte Carlo; Astrophysics; Nuclear physics; Optics; Mathematics","score_opus":0.01625586906905989,"score_gpt":0.3073320005825934,"score_spread":0.2910761315135335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052267529","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.004060274,0.000087518136,0.9927705,0.00007508567,0.0000538129,0.000037732447,0.000046661386,0.00021209962,0.0026563657],"genre_scores_gemma":[0.13504536,0.00028502406,0.85681343,0.000119758544,0.000061675935,0.0002615947,0.00016696328,0.0002300782,0.0070160185],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99970764,0.000077668774,0.000015977464,0.000039195576,0.00013287607,0.000026622825],"domain_scores_gemma":[0.99916685,0.00042259452,0.000059954084,0.0001218711,0.00016791704,0.00006087331],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076986203,0.00043723042,0.00058331876,0.00049518986,0.0006708775,0.0009179666,0.0016552946,0.0010693723,0.0038532233],"category_scores_gemma":[0.0020450389,0.00041120802,0.00076678034,0.00057214533,0.0009087273,0.0011780328,0.00084863615,0.001443283,0.00073172996],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050746043,0.00005983743,0.0005873808,0.000073675736,0.000033831177,0.00009302328,0.00008211155,0.7837128,0.0070457635,0.17128311,0.0010981328,0.035879593],"study_design_scores_gemma":[0.0000073260144,0.000004388473,0.000022735627,0.0000034370114,0.0000023957623,0.000011897091,0.0000017205252,0.99378395,0.00044472783,0.004039631,0.0016730358,0.0000047026156],"about_ca_topic_score_codex":0.0076588476,"about_ca_topic_score_gemma":0.008212008,"teacher_disagreement_score":0.0076588476,"about_ca_system_score_codex":0.00097296137,"about_ca_system_score_gemma":0.0019803839,"threshold_uncertainty_score":0.01522851},"labels":[],"label_agreement":null},{"id":"W2052275543","doi":"10.1086/496961","title":"The First Detection of Dust Emission in a High-Velocity Cloud","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Milky Way; Galactic plane; Interstellar medium; Cosmic dust; Metallicity; Dust lane; Spitzer Space Telescope; Molecular cloud; Astronomy; Infrared; Interstellar cloud; Sky; Galaxy; Telescope; Star formation; Stars","score_opus":0.006869964304456819,"score_gpt":0.2207759354222083,"score_spread":0.21390597111775148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052275543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964431,0.00031260613,0.0009685323,0.00004263105,0.000019138764,0.00001559295,0.00018993765,0.000026562573,0.0019819685],"genre_scores_gemma":[0.9989096,0.00005637786,0.00054857344,0.00003659485,0.000018384611,0.000004039615,0.00017786778,0.0000026510259,0.00024600755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986327,0.0000067508686,0.0000049967266,0.00004085374,0.00003761377,0.000046475736],"domain_scores_gemma":[0.9994062,0.000101847916,0.0001145842,0.000046786437,0.00010737462,0.0002231807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011307781,0.00019063058,0.00019136122,0.00063713535,0.00056371186,0.0006770087,0.0005023817,0.00053074065,0.0013113768],"category_scores_gemma":[0.00042662694,0.00014883479,0.00017740768,0.00041550447,0.0004141333,0.00024970347,0.00042952097,0.00031115438,0.000180506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032960172,0.00014521235,0.69237554,0.00015722282,0.00011404894,0.003025164,0.00046730659,0.00025133576,0.28630185,0.0008543374,0.0010534337,0.014924917],"study_design_scores_gemma":[0.00002069979,0.00024782616,0.9698649,0.000012032549,0.00003428415,0.0021505654,0.00014581099,0.00051614357,0.023814922,0.0002144452,0.0029690217,0.000009274636],"about_ca_topic_score_codex":0.003209775,"about_ca_topic_score_gemma":0.0051793586,"teacher_disagreement_score":0.003209775,"about_ca_system_score_codex":0.00036034037,"about_ca_system_score_gemma":0.0002477846,"threshold_uncertainty_score":0.0063821673},"labels":[],"label_agreement":null},{"id":"W2052397708","doi":"10.1086/499347","title":"Resonance Overlap Is Responsible for Ejecting Planets in Binary Systems","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Instability; Eccentricity (behavior); Planet; Boundary (topology); Resonance (particle physics); Planetary system; Celestial mechanics; Giant planet","score_opus":0.012305500196740147,"score_gpt":0.23436933056663709,"score_spread":0.22206383036989694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052397708","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99427384,0.00015448476,0.0036681297,0.00002272188,0.0000028497,0.0000041104067,0.000008545102,0.00007451909,0.0017907758],"genre_scores_gemma":[0.99956936,0.00002015377,0.00033649782,0.0000019449355,0.0000020279483,0.000001575141,0.000006148851,0.000006177946,0.000055946082],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981004,0.000021215677,0.000015418447,0.000036080208,0.00006522573,0.000052171876],"domain_scores_gemma":[0.99871004,0.00054470665,0.0004196689,0.00009667502,0.00007250187,0.0001564406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028013458,0.00020153882,0.0003686441,0.0008071843,0.0007248952,0.00086722453,0.0003668647,0.00039799314,0.0010600156],"category_scores_gemma":[0.0029288938,0.0002585987,0.00017125953,0.00028141978,0.0007223265,0.00082936476,0.0010878604,0.00022352632,0.00014362083],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014514112,0.0002254486,0.2616511,0.00044186434,0.00019088831,0.0040327995,0.0022817217,0.17563894,0.46717098,0.034503132,0.0007644771,0.051647186],"study_design_scores_gemma":[0.0001233534,0.0005050572,0.18207383,0.000055102697,0.00017457824,0.0030405119,0.0009368432,0.6626263,0.12468261,0.023723748,0.0019577174,0.00010026055],"about_ca_topic_score_codex":0.00060762605,"about_ca_topic_score_gemma":0.00046855983,"teacher_disagreement_score":0.0010600156,"about_ca_system_score_codex":0.00029967775,"about_ca_system_score_gemma":0.00016384234,"threshold_uncertainty_score":0.0035460591},"labels":[],"label_agreement":null},{"id":"W2052423194","doi":"10.1088/0004-637x/732/2/94","title":"EARLY-TYPE GALAXIES AT<i>z</i>∼ 1.3. III. ON THE DEPENDENCE OF FORMATION EPOCHS AND STAR FORMATION HISTORIES ON STELLAR MASS AND ENVIRONMENT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Centro de Astrofísica y Tecnologías Afines; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Stellar mass; Stellar population; Population; Redshift; Field galaxy; Astronomy; Star cluster; Lenticular galaxy; Galaxy cluster; Cluster (spacecraft); Redshift survey; Demography","score_opus":0.012022092864510526,"score_gpt":0.1792817437453574,"score_spread":0.16725965088084688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052423194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97638613,0.0007371592,0.0005959754,0.00038014905,0.000013637642,0.000016729724,0.001922277,0.000075999975,0.019871892],"genre_scores_gemma":[0.99612254,0.0001640739,0.00020909042,0.00006503403,0.000010643803,0.000005790137,0.00077173306,0.000007556654,0.002643423],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990237,0.0000063301013,0.0000029719815,0.000020947378,0.00001518692,0.000052274267],"domain_scores_gemma":[0.99888414,0.00019059898,0.00033764783,0.000097259624,0.00017617407,0.00031407084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000260695,0.00013677121,0.000113582166,0.0010866957,0.00034367692,0.0008497775,0.00025062845,0.00034041653,0.0061426344],"category_scores_gemma":[0.0012372142,0.00010050428,0.00023047312,0.0006047342,0.0002820034,0.00047523808,0.0004165592,0.0003152298,0.0012643345],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014398409,0.000040472496,0.9714684,0.000026038766,0.000023727565,0.000073404146,0.00037208834,0.00015343714,0.005675997,0.0025192406,0.0012895104,0.0182137],"study_design_scores_gemma":[0.0000011936174,0.00000741304,0.9985127,0.000003525503,0.0000038495773,0.000024721305,0.00009607107,0.00006752389,0.00027838297,0.00020804594,0.00079565286,9.994393e-7],"about_ca_topic_score_codex":0.015765075,"about_ca_topic_score_gemma":0.025737528,"teacher_disagreement_score":0.015765075,"about_ca_system_score_codex":0.00039595016,"about_ca_system_score_gemma":0.00021291515,"threshold_uncertainty_score":0.03134662},"labels":[],"label_agreement":null},{"id":"W2052440758","doi":"10.1088/0004-637x/762/2/94","title":"LIMITS ON THE STOCHASTIC GRAVITATIONAL WAVE BACKGROUND FROM THE NORTH AMERICAN NANOHERTZ OBSERVATORY FOR GRAVITATIONAL WAVES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":369,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Pulsar; Physics; Gravitational wave; Observatory; Gravitational wave background; Gravitational-wave observatory; Astrophysics; Supermassive black hole; Dispersion (optics); Data set; Spectral density; Astronomy; Statistics; Optics; Galaxy; Mathematics","score_opus":0.04916726047702203,"score_gpt":0.3191790870131005,"score_spread":0.27001182653607847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052440758","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872706,0.0002741228,0.0075309733,0.00019956804,0.000011792005,0.000016954144,0.002174117,0.00017138584,0.0023505648],"genre_scores_gemma":[0.9870113,0.00016563236,0.0048552933,0.000046141755,0.000034320394,0.000024476318,0.0075807944,0.00006423632,0.00021783073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99883896,0.00018216707,0.000058139194,0.00020483742,0.00062255905,0.00009340056],"domain_scores_gemma":[0.99634165,0.0009960479,0.0012296799,0.00079483655,0.0004395595,0.00019819377],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017730185,0.00036285614,0.00032866793,0.0012865277,0.0005355549,0.00067573757,0.0005749379,0.00023478745,0.00076129823],"category_scores_gemma":[0.004921628,0.00027800497,0.00034607953,0.0015596137,0.00035700417,0.0004926184,0.0009290507,0.00046393747,0.00019648441],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001823462,0.000084528445,0.9049367,0.000086840926,0.00023353905,0.0002373582,0.0004527242,0.02848931,0.019594241,0.0047055962,0.0029884344,0.03800844],"study_design_scores_gemma":[0.00001843808,0.000029849856,0.95441246,0.000013080068,0.000047994206,0.00010542108,0.000040793846,0.03707902,0.0023109592,0.0017431553,0.0041742334,0.00002447863],"about_ca_topic_score_codex":0.01548579,"about_ca_topic_score_gemma":0.033704244,"teacher_disagreement_score":0.01548579,"about_ca_system_score_codex":0.00060388807,"about_ca_system_score_gemma":0.0007796116,"threshold_uncertainty_score":0.030791283},"labels":[],"label_agreement":null},{"id":"W2052598803","doi":"10.1086/522305","title":"Ultracompact Dwarf Candidates in the Hydra Cluster","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Lernaean Hydra; Physics; Astrophysics; Dwarf galaxy; Astronomy; Photometry (optics); Cluster (spacecraft); Galaxy; Galaxy cluster; Biology; Stars; Computer science","score_opus":0.006621705081443936,"score_gpt":0.22800746016263945,"score_spread":0.2213857550811955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052598803","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991935,0.00008799351,0.00007446876,0.00001675321,0.0000018755701,0.0000029324067,0.00004341728,0.0000057161,0.0005733405],"genre_scores_gemma":[0.99925894,0.000057685254,0.0001940934,0.000014927605,0.0000033524498,0.0000030219635,0.00015750906,0.0000020360958,0.00030841274],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987125,0.000014042007,0.000006855573,0.00003360324,0.000031654414,0.00004241043],"domain_scores_gemma":[0.999524,0.00009233916,0.00012954108,0.000037410508,0.000028341723,0.00018840763],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014912273,0.00018134892,0.00025339302,0.00078624673,0.00078704435,0.0006797295,0.00024278661,0.00022654537,0.001225501],"category_scores_gemma":[0.00057528465,0.00013984955,0.00010887387,0.0005509547,0.00045611284,0.00022003519,0.0007308282,0.00020382344,0.00036322893],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026090813,0.000042221396,0.97294575,0.000027408038,0.000021725422,0.0012313086,0.0006198915,0.00021400323,0.014136228,0.0008788611,0.00043550556,0.009186157],"study_design_scores_gemma":[0.00000987483,0.0000756217,0.99205035,0.000010214149,0.00002911989,0.0021125313,0.0006770235,0.00043627984,0.002004287,0.00040178874,0.0021802762,0.000012621117],"about_ca_topic_score_codex":0.0029273457,"about_ca_topic_score_gemma":0.0067818747,"teacher_disagreement_score":0.0029273457,"about_ca_system_score_codex":0.00020836372,"about_ca_system_score_gemma":0.00016560714,"threshold_uncertainty_score":0.005820632},"labels":[],"label_agreement":null},{"id":"W2052615736","doi":"10.1086/324157","title":"Hydrostatic Expansion and Spin Changes during Type I X‐Ray Bursts","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Moment of inertia; Angular momentum; Neutron star; Hydrostatic equilibrium; Spin (aerodynamics); Atmosphere (unit); Astrophysics; Differential rotation; Rotation (mathematics); Conservation law; Computational physics; Classical mechanics; Stars; Quantum mechanics; Geometry; Thermodynamics","score_opus":0.015982253814417098,"score_gpt":0.2943691888160681,"score_spread":0.278386935001651,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052615736","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973814,0.000083620274,0.0012086864,0.000031231033,0.000007803173,0.0000037912084,0.000060315186,0.00005360969,0.0011694367],"genre_scores_gemma":[0.99938655,0.000065329,0.00025957904,0.000005749256,0.000005350878,0.0000041199196,0.000059498383,0.000015003847,0.00019883057],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995637,0.000007832411,0.0000027090841,0.000007720842,0.000007803781,0.000017571321],"domain_scores_gemma":[0.99968576,0.00009944481,0.00011480924,0.000025963882,0.000017953056,0.0000561447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001382094,0.00032367156,0.00017601474,0.00026201963,0.00031486244,0.00043234104,0.00034656603,0.00035355554,0.000875047],"category_scores_gemma":[0.0012402831,0.00025472138,0.0005167567,0.00024259547,0.00042816476,0.0003323111,0.00037790783,0.00033861882,0.00015130658],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007152822,0.00009233828,0.23421568,0.00009384091,0.00015973901,0.0013865301,0.000359324,0.7151756,0.029323922,0.005318135,0.00050795387,0.012651733],"study_design_scores_gemma":[0.00011697797,0.0002512461,0.19456707,0.00001509666,0.000102449456,0.00035853474,0.0001310121,0.7931993,0.008251664,0.0020978625,0.00085959636,0.000049212354],"about_ca_topic_score_codex":0.006656667,"about_ca_topic_score_gemma":0.0025431484,"teacher_disagreement_score":0.006656667,"about_ca_system_score_codex":0.00046457138,"about_ca_system_score_gemma":0.00015932656,"threshold_uncertainty_score":0.013235867},"labels":[],"label_agreement":null},{"id":"W2052656417","doi":"10.1086/521780","title":"A 1.4 GHz Arecibo Survey for Pulsars in Globular Clusters","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Globular cluster; Pulsar; Physics; Millisecond pulsar; Astrophysics; Astronomy; Population; X-ray pulsar; Galaxy","score_opus":0.0214913053941381,"score_gpt":0.34823415084480464,"score_spread":0.32674284545066656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052656417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99381566,0.00058281265,0.0005682825,0.00020043792,0.000009206182,0.000037693073,0.0015803379,0.00004191386,0.0031636748],"genre_scores_gemma":[0.9826828,0.0016126003,0.003411891,0.00017298604,0.00006523244,0.00004967243,0.007702961,0.0000276319,0.0042742346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997235,0.000034321933,0.000010110501,0.000062325504,0.00007841666,0.000091249385],"domain_scores_gemma":[0.9991223,0.00009181146,0.0002606519,0.00007458655,0.00023597864,0.00021478294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004938323,0.00028841197,0.00025946432,0.0028828431,0.000816503,0.00046106277,0.0003179077,0.00026457943,0.0020701175],"category_scores_gemma":[0.0008489225,0.00017704065,0.0001466006,0.003182904,0.0002293969,0.00041213774,0.00057722896,0.00029748303,0.00056236703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007229132,0.00008502238,0.9656699,0.000050763807,0.000028951943,0.00012565864,0.0007589509,0.00012938057,0.00943045,0.00019993233,0.0021054684,0.021343201],"study_design_scores_gemma":[0.000003924883,0.000024048533,0.9958759,0.000006653962,0.0000095088,0.00009937496,0.00016380489,0.00007479392,0.00030061402,0.000025514226,0.0034127552,0.0000031913823],"about_ca_topic_score_codex":0.027126145,"about_ca_topic_score_gemma":0.046998244,"teacher_disagreement_score":0.027126145,"about_ca_system_score_codex":0.0005078439,"about_ca_system_score_gemma":0.00045449764,"threshold_uncertainty_score":0.05393648},"labels":[],"label_agreement":null},{"id":"W2052937997","doi":"10.1086/510584","title":"High-Resolution Spectra of Carbon Nanoparticles: Laboratory Simulation of the Infrared Emission Features Associated with Polycyclic Aromatic Hydrocarbons","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Carbon Nanotubes in Composites","field":"Materials Science","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Infrared; Infrared spectroscopy; Spectral line; Spectral resolution; Carbon fibers; Raman spectroscopy; Wavelength; Emission spectrum; Physics; Analytical Chemistry (journal); Spectroscopy; Astrochemistry; Molecular cloud; Astrophysics; Interstellar medium; Materials science; Chemistry; Optics; Astronomy; Stars; Organic chemistry; Composite number","score_opus":0.004641583939502117,"score_gpt":0.20844668940193625,"score_spread":0.20380510546243413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052937997","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99239576,0.000042245367,0.005733191,0.00003835883,0.000008711582,0.000011123215,0.000064130116,0.00008731915,0.0016191687],"genre_scores_gemma":[0.9960561,0.00003012029,0.0035221009,0.0000076773595,0.000002250663,0.000015392203,0.00006889207,0.000018826897,0.0002785997],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994135,0.000007652026,0.0000020009459,0.000012591946,0.000022745948,0.000013633175],"domain_scores_gemma":[0.9997925,0.00011017062,0.000023605171,0.000021326185,0.000037711172,0.000014730014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017731484,0.00021867677,0.00021539912,0.000160003,0.00020253166,0.0002652432,0.000387727,0.00039803926,0.0008391368],"category_scores_gemma":[0.00046823677,0.00015286785,0.00028524912,0.00015114911,0.00029694833,0.00026721493,0.00016215046,0.00031510956,0.000082087216],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016832416,0.0002465365,0.0047261394,0.00008974121,0.000052472536,0.0003195363,0.00011446233,0.78745234,0.19861987,0.0022024312,0.000363178,0.0056450027],"study_design_scores_gemma":[0.000017885706,0.00008664453,0.0012766103,0.0000021754634,0.000005944146,0.000024764726,0.000023049319,0.9656685,0.032395102,0.00027154502,0.00021706641,0.000010587939],"about_ca_topic_score_codex":0.003227797,"about_ca_topic_score_gemma":0.0022967008,"teacher_disagreement_score":0.003227797,"about_ca_system_score_codex":0.00051575806,"about_ca_system_score_gemma":0.00024334746,"threshold_uncertainty_score":0.0064180493},"labels":[],"label_agreement":null},{"id":"W2052950672","doi":"10.1086/378224","title":"Scattered Light from Close‐in Extrasolar Planets: Prospects of Detection with the<i>MOST</i>Satellite","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Light curve; Exoplanet; Planet; Orbital inclination; Light scattering; Amplitude; Planetary system; Angular diameter; Angular resolution (graph drawing)","score_opus":0.0055867853051339705,"score_gpt":0.18943878360920516,"score_spread":0.18385199830407117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052950672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970445,0.000049869643,0.0015233428,0.00021762148,0.000005634141,0.0000074765985,0.00011825862,0.00005650572,0.0009767144],"genre_scores_gemma":[0.9986047,0.00002893624,0.0010231801,0.000020629981,0.0000034193872,0.0000045175916,0.00017763027,0.000012205084,0.00012477713],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983656,0.00006018028,0.000004654398,0.000032362354,0.000033818458,0.00003241585],"domain_scores_gemma":[0.99882835,0.000662153,0.00012588882,0.00009245599,0.00015879968,0.00013236463],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009272701,0.00040063245,0.00037739478,0.0002728928,0.0004956427,0.00069316005,0.00064356293,0.00089519966,0.0005729634],"category_scores_gemma":[0.0022246314,0.00035401492,0.00057828985,0.00039429494,0.0006814831,0.00071622897,0.00045968086,0.00060257915,0.00008654915],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017309374,0.00013301092,0.084379695,0.000024195639,0.00008173968,0.000088206354,0.00007690751,0.9090243,0.0013286007,0.0017436061,0.00057570095,0.0023708225],"study_design_scores_gemma":[0.000057712157,0.00009772182,0.01704086,0.000007017516,0.00002134167,0.00003715106,0.00004351061,0.98004824,0.0015945205,0.00074637943,0.0002892849,0.000016271135],"about_ca_topic_score_codex":0.03317938,"about_ca_topic_score_gemma":0.02035975,"teacher_disagreement_score":0.03317938,"about_ca_system_score_codex":0.0012149521,"about_ca_system_score_gemma":0.00066099275,"threshold_uncertainty_score":0.06597251},"labels":[],"label_agreement":null},{"id":"W2052958709","doi":"10.1086/524771","title":"Cosmic‐Ray Propagation: Nonlinear Diffusion Parallel and Perpendicular to Mean Magnetic Field","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Cosmic ray; Turbulence; Magnetic field; Astrophysics; Computational physics; Magnetohydrodynamic turbulence; Mean free path; Scattering; Classical mechanics; Mechanics; Magnetohydrodynamics; Optics; Quantum mechanics","score_opus":0.006280095848264865,"score_gpt":0.21064942626855557,"score_spread":0.2043693304202907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052958709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5037477,0.003065215,0.4399621,0.002363045,0.00034375887,0.00008978345,0.00032488603,0.00028770216,0.049815852],"genre_scores_gemma":[0.96738917,0.00164166,0.018506387,0.0001368091,0.00012295927,0.000044482982,0.0001179295,0.00006826603,0.011972364],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998807,0.00003153503,0.0000052626397,0.000025327776,0.000025382064,0.000031770818],"domain_scores_gemma":[0.99957174,0.00014333038,0.00013814057,0.000027606624,0.000072309864,0.000046901365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033836422,0.0005973487,0.00037731332,0.00054777967,0.0005958842,0.0013112274,0.0007480023,0.0010218716,0.0013077522],"category_scores_gemma":[0.0015283178,0.00032239748,0.0007003633,0.00053235004,0.0014242275,0.0013124213,0.0009460787,0.0007718476,0.00022623432],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007745566,0.00006171989,0.0058018365,0.00009079922,0.000054133292,0.0005324539,0.00020580852,0.665281,0.008287786,0.3133656,0.00094135344,0.0053000543],"study_design_scores_gemma":[0.000011800939,0.000012366087,0.00064213766,0.0000047573417,0.000006282015,0.000060857044,0.000016231152,0.98274577,0.0003148777,0.015735954,0.00043904327,0.000010045718],"about_ca_topic_score_codex":0.021822067,"about_ca_topic_score_gemma":0.0059611113,"teacher_disagreement_score":0.021822067,"about_ca_system_score_codex":0.001256104,"about_ca_system_score_gemma":0.0010872046,"threshold_uncertainty_score":0.043390095},"labels":[],"label_agreement":null},{"id":"W2052993259","doi":"10.1088/0004-637x/732/2/71","title":"A POWERFUL AGN OUTBURST IN RBS 797","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Accretion (finance); Luminosity; Galaxy; Active galactic nucleus; Intracluster medium; Surface brightness; Cooling flow; Observatory; Star formation; Line-of-sight; Astronomy; Cluster (spacecraft); Galaxy cluster","score_opus":0.01145702828116504,"score_gpt":0.20806449004826913,"score_spread":0.19660746176710409,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2052993259","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988695,0.000058651654,0.00006881062,0.000014423517,0.0000032388032,0.0000041921303,0.0001369984,0.000030871193,0.00081335695],"genre_scores_gemma":[0.9986848,0.000044178967,0.00022370998,0.000020560494,0.000009904266,0.000004390187,0.0006593356,0.000011100771,0.00034204393],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987495,0.0000057330617,0.0000051326133,0.000031046064,0.000035689798,0.000047448844],"domain_scores_gemma":[0.999696,0.000022899581,0.00008370738,0.00002966644,0.000033342792,0.00013445054],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110644614,0.00025760036,0.0004661699,0.00077651197,0.0008184189,0.00050941453,0.00041207662,0.00031378813,0.0008115511],"category_scores_gemma":[0.0002021115,0.00014128062,0.00026570386,0.00049521367,0.00025070301,0.00010831737,0.0006850146,0.00025287436,0.00050131377],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045194922,0.0002001292,0.763398,0.00008469964,0.00010779647,0.0069463104,0.0014125819,0.0011276813,0.20944545,0.0005826325,0.0017436531,0.014499175],"study_design_scores_gemma":[0.000016246013,0.0001691868,0.9896667,0.000009935565,0.000043806675,0.0021534453,0.00027984544,0.0014076983,0.00392868,0.00010149906,0.0022059334,0.000017062803],"about_ca_topic_score_codex":0.009743094,"about_ca_topic_score_gemma":0.016441982,"teacher_disagreement_score":0.009743094,"about_ca_system_score_codex":0.0006321146,"about_ca_system_score_gemma":0.00024502535,"threshold_uncertainty_score":0.019372761},"labels":[],"label_agreement":null},{"id":"W2053125503","doi":"10.1086/520913","title":"Speckle Noise and Dynamic Range in Coronagraphic Images","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Coronagraph; Speckle pattern; Starlight; Adaptive optics; Physics; Speckle noise; Optics; Context (archaeology); Exoplanet; Residual; High dynamic range; Wavefront; Dynamic range; Computer science; Astronomy; Algorithm; Planet","score_opus":0.0068012326567298935,"score_gpt":0.2331636754283849,"score_spread":0.22636244277165501,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053125503","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5668789,0.012184725,0.015771642,0.06835792,0.051435158,0.0005100878,0.002655274,0.0026148467,0.27959156],"genre_scores_gemma":[0.7009232,0.0040514506,0.005930585,0.0018942492,0.015811892,0.00009086983,0.0019185852,0.00088338315,0.26849574],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.997888,0.00024424333,0.00012512904,0.00019570442,0.0014303839,0.000116575255],"domain_scores_gemma":[0.9679002,0.0035501586,0.0013659481,0.001210261,0.024169208,0.0018042651],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002134632,0.00024692804,0.0006604997,0.00245485,0.0010306009,0.0021524562,0.00053372845,0.0016974146,0.040343814],"category_scores_gemma":[0.030318545,0.00028887484,0.00021981123,0.0009834279,0.000577467,0.0013777615,0.0007148015,0.0004920599,0.014106409],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010187102,0.00016830108,0.044028033,0.0013986656,0.00010121566,0.0015807272,0.000697748,0.0015600711,0.040109403,0.0064957486,0.46472064,0.43812075],"study_design_scores_gemma":[0.00028039687,0.000485705,0.33481592,0.00060570915,0.00019951552,0.0049029593,0.0014345814,0.022745518,0.04868216,0.013470182,0.57215124,0.00022611413],"about_ca_topic_score_codex":0.00057426706,"about_ca_topic_score_gemma":0.0013398571,"teacher_disagreement_score":0.040343814,"about_ca_system_score_codex":0.00053147954,"about_ca_system_score_gemma":0.00054116035,"threshold_uncertainty_score":0.13496351},"labels":[],"label_agreement":null},{"id":"W2053137705","doi":"10.1086/367786","title":"Constraints on the Ionization Balance of Hot‐Star Winds from<i>FUSE</i>Observations of O Stars in the Large Magellanic Cloud","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Stars; Ionization; Large Magellanic Cloud; O-type star; Balance (ability); Spectral line; Cloud computing","score_opus":0.016323352288462996,"score_gpt":0.2195405914100165,"score_spread":0.2032172391215535,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053137705","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936673,0.0004816606,0.0006235586,0.00018019827,0.000019847166,0.000005206994,0.0006511643,0.000037250684,0.004333755],"genre_scores_gemma":[0.99840003,0.00018203822,0.00018694413,0.000068977315,0.00002733258,0.0000015101258,0.00076832355,0.000016501263,0.0003483706],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997886,0.00001739857,0.000014988268,0.000044813496,0.00007095297,0.0000632481],"domain_scores_gemma":[0.9988721,0.00036679307,0.00030226816,0.000074857155,0.00021322277,0.00017080708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056098157,0.00050078105,0.00041034754,0.0009780066,0.00063521334,0.0015835153,0.00044710975,0.00095580245,0.0036237766],"category_scores_gemma":[0.0022402508,0.0005030044,0.00024319251,0.0005089112,0.00029307007,0.0011386295,0.0005393598,0.00039234612,0.0007516806],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009870606,0.00007591622,0.7849081,0.0001590158,0.00028949502,0.0004197359,0.00034540365,0.0029232858,0.18855204,0.0019014148,0.001826112,0.017612446],"study_design_scores_gemma":[0.0000563783,0.000043782482,0.98382264,0.000026234,0.00010035597,0.0001809333,0.00019166492,0.0043568616,0.008750686,0.0011186114,0.0013293864,0.000022394383],"about_ca_topic_score_codex":0.00693647,"about_ca_topic_score_gemma":0.013844567,"teacher_disagreement_score":0.00693647,"about_ca_system_score_codex":0.00049240736,"about_ca_system_score_gemma":0.00027857674,"threshold_uncertainty_score":0.013792157},"labels":[],"label_agreement":null},{"id":"W2053137720","doi":"10.1086/320264","title":"Two Young Radio Pulsars Coincident with EGRET Sources","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Egret; Physics; Pulsar; Astrophysics; Observatory; Astronomy; Dipole; Magnetic field; Magnetic dipole; Gamma ray","score_opus":0.0100797945625653,"score_gpt":0.29836241898613614,"score_spread":0.28828262442357083,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053137720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970285,0.00047400617,0.00079726026,0.00008062185,0.000033164386,0.00001280087,0.00022863205,0.000039080398,0.0013059807],"genre_scores_gemma":[0.9961515,0.00024594206,0.0014773759,0.00017280734,0.000055920926,0.000014765968,0.00093462697,0.0000093457875,0.00093771337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998103,0.00001550489,0.000018222416,0.00005608159,0.000041268606,0.00005865826],"domain_scores_gemma":[0.9990988,0.000106084444,0.0003978081,0.000105897234,0.00009681905,0.00019464985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000259333,0.00027203423,0.00031408804,0.0011110425,0.00044896203,0.0009237143,0.00030785898,0.00064826105,0.0005844237],"category_scores_gemma":[0.0009719469,0.00020800483,0.000157612,0.0007192834,0.00031873348,0.0003605938,0.00095670903,0.00030307568,0.00033511937],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057608396,0.00014766345,0.9093814,0.00006244521,0.00007077366,0.012414765,0.0013348223,0.0002546937,0.041836593,0.0016743045,0.0009248024,0.031321622],"study_design_scores_gemma":[0.00003688027,0.0002351477,0.97068226,0.000018524095,0.000057198573,0.010418921,0.00026963753,0.00042481063,0.005973801,0.0005631013,0.011298958,0.000020876498],"about_ca_topic_score_codex":0.00088540826,"about_ca_topic_score_gemma":0.0011761783,"teacher_disagreement_score":0.0011110425,"about_ca_system_score_codex":0.00025464589,"about_ca_system_score_gemma":0.00011920656,"threshold_uncertainty_score":0.001955092},"labels":[],"label_agreement":null},{"id":"W2053241862","doi":"10.1086/381229","title":"Discovery of Another Peculiar Radial Distribution of Blue Stragglers in Globular Clusters: The Case of 47 Tucanae","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Blue straggler; Bimodality; Cluster (spacecraft); Star cluster; Stars; Hubble space telescope; Horizontal branch","score_opus":0.007966642066763214,"score_gpt":0.2178734481695288,"score_spread":0.2099068061027656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053241862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99945253,0.00004349958,0.000100377176,0.000013694331,6.05037e-7,0.0000015251879,0.000051832216,0.0000061629307,0.00032966406],"genre_scores_gemma":[0.9992372,0.000047779457,0.00031559955,0.000008079956,0.0000020126668,0.000001878158,0.00017424858,0.0000054763354,0.00020772193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998259,0.000011855601,0.000006534865,0.000044411867,0.000037744347,0.00007358821],"domain_scores_gemma":[0.99937016,0.00007341486,0.00014015823,0.000108011904,0.00019558186,0.0001126739],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028907432,0.00012838775,0.00024638034,0.002518296,0.0010125606,0.00079614524,0.00039469506,0.0002858099,0.000681287],"category_scores_gemma":[0.0011478355,0.00012501274,0.00013960678,0.0021511721,0.0007760678,0.0002778349,0.00075697,0.00019678139,0.00012064217],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000082445884,0.000013539485,0.9689538,0.000011568539,0.000031951542,0.0005476074,0.0013547707,0.00043049618,0.013745799,0.00033243044,0.00017477579,0.014320835],"study_design_scores_gemma":[0.0000023544105,0.000017512044,0.9950245,0.0000055193077,0.000015980184,0.00051537046,0.0005655062,0.0007154913,0.0018347285,0.00013633224,0.0011567549,0.000009928815],"about_ca_topic_score_codex":0.12044026,"about_ca_topic_score_gemma":0.1709123,"teacher_disagreement_score":0.12044026,"about_ca_system_score_codex":0.00074290315,"about_ca_system_score_gemma":0.00065014354,"threshold_uncertainty_score":0.23947841},"labels":[],"label_agreement":null},{"id":"W2053251397","doi":"10.1088/0004-637x/756/2/190","title":"GRB 120422A: A LOW-LUMINOSITY GAMMA-RAY BURST DRIVEN BY A CENTRAL ENGINE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Gamma-ray burst; Astrophysics; Physics; Supernova; Luminosity; Light curve; Shock (circulatory); Lorentz factor; Curvature; Astronomy; Galaxy; Lorentz transformation; Geometry","score_opus":0.007299018200969913,"score_gpt":0.21144024532305888,"score_spread":0.20414122712208896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053251397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99378973,0.00046593996,0.0010006105,0.0000338768,0.00001782562,0.00003470756,0.0011816814,0.00022259394,0.0032530816],"genre_scores_gemma":[0.99389315,0.00017251342,0.0011025871,0.000043137203,0.00004149679,0.00001937307,0.0038372255,0.000034139735,0.0008564045],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983335,0.000015263578,0.000019855697,0.000035184712,0.000055805074,0.000040520415],"domain_scores_gemma":[0.9994912,0.000057003454,0.00025236976,0.00005894748,0.000039320134,0.000101171834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025426742,0.00084189593,0.00041653024,0.0011844661,0.000515484,0.0012295317,0.00041105147,0.0006098287,0.0024293442],"category_scores_gemma":[0.00067043037,0.00018324249,0.00034769633,0.0013248931,0.0003880245,0.0003707077,0.0007706371,0.0003979243,0.00087536895],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014236722,0.00037945877,0.7964467,0.00044530295,0.00024410224,0.0067117107,0.0003651092,0.0033041744,0.13122495,0.0025618793,0.0058891512,0.051003795],"study_design_scores_gemma":[0.00006304392,0.00026381825,0.97230655,0.000023794373,0.000049836137,0.007918075,0.00014498933,0.0040708077,0.007286087,0.00079081545,0.007056451,0.000025610107],"about_ca_topic_score_codex":0.0010960611,"about_ca_topic_score_gemma":0.0017656416,"teacher_disagreement_score":0.0024293442,"about_ca_system_score_codex":0.00022570902,"about_ca_system_score_gemma":0.000111179026,"threshold_uncertainty_score":0.0081269145},"labels":[],"label_agreement":null},{"id":"W2053292882","doi":"10.1086/521621","title":"A Subaru Weak‐Lensing Survey. I. Cluster Candidates and Spectroscopic Verification","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Halo; Astrophysics; Subaru Telescope; Weak gravitational lensing; Redshift; Galaxy; Intracluster medium; Galaxy cluster; Astronomy; Cluster (spacecraft); Spectrograph; Spectral line; Computer science","score_opus":0.008217713572770222,"score_gpt":0.226575318365888,"score_spread":0.21835760479311778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053292882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99000704,0.00031443065,0.0004694377,0.000059287755,0.0000071585478,0.00007986916,0.005931089,0.00008420882,0.0030474965],"genre_scores_gemma":[0.9699873,0.00038412717,0.0039187474,0.00008765443,0.0000457517,0.00011616247,0.021248957,0.000059951366,0.004151395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996087,0.00006352662,0.00003123902,0.000068739704,0.00012592255,0.00010188497],"domain_scores_gemma":[0.9984794,0.00009344007,0.0003250176,0.00027685612,0.00034629073,0.00047900862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007903392,0.00029242923,0.00027682324,0.004316206,0.00072948454,0.0004982962,0.00044997726,0.0002376015,0.003424523],"category_scores_gemma":[0.0008712125,0.0002247084,0.00023744097,0.0022780707,0.00020090415,0.00043275586,0.0010579692,0.00018655081,0.0031283572],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030227078,0.00011042553,0.9565927,0.00006664133,0.00003713977,0.0003792898,0.0010477726,0.0001695283,0.01047093,0.00038698997,0.003721323,0.02671498],"study_design_scores_gemma":[0.00000775592,0.00010024218,0.9933461,0.0000065728796,0.0000117358095,0.0002584285,0.0002766754,0.00029085315,0.00078060385,0.000046166686,0.0048685907,0.0000063744696],"about_ca_topic_score_codex":0.009366423,"about_ca_topic_score_gemma":0.014401788,"teacher_disagreement_score":0.009366423,"about_ca_system_score_codex":0.00025820205,"about_ca_system_score_gemma":0.0003991383,"threshold_uncertainty_score":0.018623829},"labels":[],"label_agreement":null},{"id":"W2053418998","doi":"10.1088/0004-637x/769/2/122","title":"SERENDIPITOUS DISCOVERY OF AN INFRARED BOW SHOCK NEAR PSR J1549–4848 WITH<i>SPITZER</i>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Nebula; Astrophysics; Pulsar wind nebula; Astronomy; Bow shock (aerodynamics); Stars; Proper motion; Sky; Orion Nebula; Infrared; Shock wave","score_opus":0.005748708109193312,"score_gpt":0.2101539613422108,"score_spread":0.20440525323301748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053418998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988336,0.00009051236,0.00016455451,0.000034054483,0.000004761347,0.0000026766722,0.00002792049,0.000020809128,0.00082127954],"genre_scores_gemma":[0.99929285,0.000044211596,0.00028050615,0.000043172116,0.000018865916,0.0000032694595,0.00007959651,0.0000039983825,0.00023349289],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990666,0.0000063463526,0.0000055623964,0.000030357072,0.000025536414,0.000025571899],"domain_scores_gemma":[0.9997062,0.000020587137,0.00015627648,0.000029987976,0.000031502448,0.00005553578],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001625965,0.00017530574,0.00018707736,0.0006241008,0.0004282807,0.0004457129,0.00029983465,0.00039417992,0.0010653595],"category_scores_gemma":[0.00035257303,0.00012482345,0.00015004714,0.00029843237,0.0003752933,0.00032273235,0.00056699757,0.00026448714,0.00036882865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023172754,0.00007075835,0.8397132,0.00003578763,0.000059552916,0.0035904904,0.0005893645,0.00014552384,0.13964035,0.0002757494,0.00066201534,0.014985481],"study_design_scores_gemma":[0.000008122953,0.00015443857,0.9854892,0.0000076719325,0.000034018896,0.0030596254,0.00020133982,0.00022179382,0.008487442,0.00011908712,0.0022116734,0.0000055504033],"about_ca_topic_score_codex":0.0009451966,"about_ca_topic_score_gemma":0.0015639218,"teacher_disagreement_score":0.0010653595,"about_ca_system_score_codex":0.00018747163,"about_ca_system_score_gemma":0.00007287365,"threshold_uncertainty_score":0.0035640001},"labels":[],"label_agreement":null},{"id":"W2053460843","doi":"10.1086/504895","title":"Collapse of Neutron Stars to Black Holes in Binary Systems: A Model for Short Gamma-Ray Bursts","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Neutron star; Globular cluster; Roche lobe; X-ray binary; Stellar black hole; Accretion (finance); Binary star; X-ray burster; Binary black hole; Black hole (networking)","score_opus":0.01447688582394986,"score_gpt":0.24229708419418858,"score_spread":0.22782019837023873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053460843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8689295,0.0025274025,0.07054262,0.003789134,0.0003823034,0.00027584773,0.0004643215,0.0005130471,0.052575722],"genre_scores_gemma":[0.9752102,0.0013367228,0.00425859,0.0004376947,0.0003732345,0.00018394571,0.00018576239,0.00012496604,0.01788883],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99965656,0.00010304263,0.000021140526,0.00006064645,0.00006109034,0.00009751221],"domain_scores_gemma":[0.99847406,0.00038928585,0.00037098513,0.00010846334,0.00012549743,0.0005316915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011497599,0.0010613272,0.0015332169,0.0012574189,0.0019516132,0.0038252631,0.0029624936,0.003634194,0.0075837052],"category_scores_gemma":[0.003654283,0.0008335118,0.0015908963,0.00068326655,0.0023909516,0.0036193253,0.002956362,0.0014848913,0.0024157902],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007998299,0.00064447394,0.027050022,0.0002826814,0.00020907725,0.004283603,0.0025196522,0.3366524,0.009787907,0.59659976,0.0065885396,0.014582053],"study_design_scores_gemma":[0.00036744092,0.00022002734,0.0042101447,0.00004930753,0.00006826701,0.0008935327,0.0002901695,0.79537857,0.00026789217,0.19529468,0.0028927056,0.000067347275],"about_ca_topic_score_codex":0.007062602,"about_ca_topic_score_gemma":0.0035980411,"teacher_disagreement_score":0.0075837052,"about_ca_system_score_codex":0.0015890668,"about_ca_system_score_gemma":0.0008015801,"threshold_uncertainty_score":0.025370002},"labels":[],"label_agreement":null},{"id":"W2053556981","doi":"10.1086/430668","title":"Long-Term Variations in the Pulse Emission from PSR J0737-3039B","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Astrophysics; Physics; Radio telescope; Pulse (music); Precession; Longitude; Modulation (music); Telescope; Astronomy; Variation (astronomy); Orbital period; Term (time); Geodesy; Optics; Geology; Stars; Latitude","score_opus":0.014059255615050906,"score_gpt":0.32417071572772144,"score_spread":0.31011146011267055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053556981","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99384284,0.00031015984,0.00019749356,0.00011898642,0.00003235251,0.000012896597,0.0031410558,0.00004743174,0.0022968636],"genre_scores_gemma":[0.99159724,0.000119481745,0.0001962254,0.00007050035,0.00002668926,0.000034866636,0.006024814,0.000030660467,0.001899474],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999218,0.0000048957627,0.0000038000385,0.000022767877,0.000023345197,0.0000234032],"domain_scores_gemma":[0.9996904,0.000055435634,0.000050285944,0.000029674,0.00008412633,0.000090043235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022164769,0.00020309459,0.00023841643,0.0003844707,0.00040310572,0.00034140015,0.00024317535,0.00045532067,0.0031553693],"category_scores_gemma":[0.00042496747,0.00014890818,0.00018519361,0.0005558316,0.00018761719,0.000312778,0.00031187042,0.00057545985,0.0010591515],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020020413,0.00062789227,0.38682908,0.00027341573,0.00043134493,0.0006014601,0.00042512963,0.001033845,0.55972993,0.0005990265,0.007204876,0.04024196],"study_design_scores_gemma":[0.000013171115,0.00004443365,0.9960896,0.000008486556,0.000022443397,0.00006842341,0.000032081916,0.0004153089,0.0022692846,0.00004809397,0.0009833314,0.000005447747],"about_ca_topic_score_codex":0.007013333,"about_ca_topic_score_gemma":0.013486687,"teacher_disagreement_score":0.007013333,"about_ca_system_score_codex":0.0004026034,"about_ca_system_score_gemma":0.0002355963,"threshold_uncertainty_score":0.0139449835},"labels":[],"label_agreement":null},{"id":"W2053619969","doi":"10.1088/0004-637x/709/1/191","title":"THE DISRUPTION OF GIANT MOLECULAR CLOUDS BY RADIATION PRESSURE &amp; THE EFFICIENCY OF STAR FORMATION IN GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":463,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Luminous infrared galaxy; Astronomy; Supernova; Redshift; Molecular cloud; Stars; Radiation pressure; Milky Way; Peculiar galaxy; Disc galaxy","score_opus":0.005646949654009445,"score_gpt":0.23465767904352486,"score_spread":0.22901072938951542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053619969","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961234,0.00033391174,0.00058326893,0.000084539635,0.0000031313405,0.000003525005,0.00009056002,0.00004230266,0.002735475],"genre_scores_gemma":[0.99955505,0.00007559779,0.000103897124,0.000013570143,0.0000031007655,0.0000017834989,0.00004020091,0.0000022722927,0.00020455758],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99989486,0.000013166495,0.000004779251,0.0000224265,0.000024326746,0.00004049977],"domain_scores_gemma":[0.99954635,0.000053321986,0.00027219445,0.00003100941,0.000023226485,0.00007386557],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014674368,0.00027465387,0.00017389366,0.00031627493,0.00034781752,0.0011201975,0.00043972326,0.0003997529,0.0014743683],"category_scores_gemma":[0.0006761015,0.00020598895,0.00030507133,0.00036518683,0.00053979596,0.00050149614,0.00047849992,0.00015867903,0.00020958632],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009535379,0.00009940903,0.89620703,0.000094710944,0.00013887185,0.00053511106,0.00021842879,0.02973387,0.05150496,0.0059704264,0.0009865477,0.014415317],"study_design_scores_gemma":[0.000014615704,0.000086745655,0.95638525,0.000011396265,0.00003318048,0.0003331047,0.00016070598,0.033703797,0.005494674,0.0021658533,0.0015985245,0.000012044193],"about_ca_topic_score_codex":0.0046707876,"about_ca_topic_score_gemma":0.003703982,"teacher_disagreement_score":0.0046707876,"about_ca_system_score_codex":0.0006050844,"about_ca_system_score_gemma":0.00017633424,"threshold_uncertainty_score":0.009287238},"labels":[],"label_agreement":null},{"id":"W2053644183","doi":"10.1088/0004-637x/779/1/61","title":"EXTRAGALACTIC MILLIMETER-WAVE POINT-SOURCE CATALOG, NUMBER COUNTS AND STATISTICS FROM 771 deg<sup>2</sup>OF THE SPT-SZ SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University; Canadian Institute for Theoretical Astrophysics; Dalhousie University","funders":"Jet Propulsion Laboratory; Science and Technology Facilities Council; European Commission; National Aeronautics and Space Administration; California Institute of Technology; Japan Aerospace Exploration Agency; Gordon and Betty Moore Foundation; University of California, Los Angeles; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Source counts; Astronomy; Redshift; Point source; Population; Millimeter; South Pole Telescope; Synchrotron; Active galactic nucleus; Brightness; Optics","score_opus":0.010574016927597478,"score_gpt":0.20470467696628977,"score_spread":0.19413066003869228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053644183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7289611,0.00045611712,0.003067782,0.00012527058,0.00003130985,0.00014180416,0.25175142,0.0004185294,0.015046717],"genre_scores_gemma":[0.41085428,0.0007822367,0.0034839974,0.00007033698,0.00008823664,0.00025044347,0.57828283,0.00012224616,0.00606539],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967754,0.000031821273,0.0000342861,0.00005384591,0.00014299287,0.000059482063],"domain_scores_gemma":[0.99867284,0.00017102073,0.00038371395,0.00025095904,0.00031785123,0.00020366316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004158609,0.00036500688,0.00037141817,0.0038205525,0.00022570818,0.00046687922,0.00060849974,0.00014568312,0.009871929],"category_scores_gemma":[0.0012585141,0.00013481834,0.00017397391,0.005544183,0.0001466448,0.0003690256,0.00066704553,0.00022443607,0.005051263],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021071949,0.000077181074,0.8714459,0.00022635919,0.00012970815,0.00023855978,0.0002970584,0.0020335892,0.004065385,0.0014411687,0.05855113,0.061283175],"study_design_scores_gemma":[0.00002671626,0.000033625678,0.9721863,0.000013233039,0.000028251541,0.0002833907,0.00012187296,0.0010774983,0.00083035347,0.00017364892,0.025218245,0.000006837154],"about_ca_topic_score_codex":0.008289116,"about_ca_topic_score_gemma":0.0098346,"teacher_disagreement_score":0.009871929,"about_ca_system_score_codex":0.00042519643,"about_ca_system_score_gemma":0.00042221375,"threshold_uncertainty_score":0.033024907},"labels":[],"label_agreement":null},{"id":"W2053668962","doi":"10.1086/594364","title":"A Massive Core in Jupiter Predicted from First-Principles Simulations","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":256,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Engineering and Physical Sciences Research Council; Natural Sciences and Engineering Research Council of Canada; Dalhousie University; Western Canada Research Grid; National Aeronautics and Space Administration; National Science Foundation","keywords":"Jovian; Jupiter (rocket family); Observable; Accretion (finance); Planetary science; Planet; Core (optical fiber); Equation of state; Gas giant","score_opus":0.026028461877905695,"score_gpt":0.22451538112117403,"score_spread":0.19848691924326833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053668962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9658016,0.0001543505,0.0066325977,0.0004125347,0.000031829317,0.000057360456,0.00075074256,0.00032476475,0.025834186],"genre_scores_gemma":[0.99385816,0.00008504899,0.0038852412,0.00009380807,0.000011115876,0.00007233684,0.00037973453,0.00006393666,0.0015506065],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998956,0.00002572498,0.000003028131,0.000015921873,0.00002585309,0.00003387495],"domain_scores_gemma":[0.9994746,0.0002447399,0.00006067827,0.00004060795,0.000080928476,0.000098589604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003913538,0.0004447196,0.00066588284,0.00057986425,0.0009010364,0.0009661295,0.0008662352,0.0010734628,0.0027234177],"category_scores_gemma":[0.0018566542,0.00042077896,0.00053039147,0.0004144688,0.000947211,0.0006244156,0.0004950355,0.0005989984,0.00023005728],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008910152,0.000064116735,0.0054995725,0.000045556546,0.000024265193,0.00015151594,0.00011426654,0.97960496,0.0010139132,0.010641716,0.0011201167,0.0016309029],"study_design_scores_gemma":[0.00005347998,0.00002465287,0.0014481071,0.0000056621348,0.0000068586105,0.000014183384,0.00002605248,0.99524057,0.00014293815,0.0027632136,0.00026800088,0.0000061723404],"about_ca_topic_score_codex":0.022281833,"about_ca_topic_score_gemma":0.012490045,"teacher_disagreement_score":0.022281833,"about_ca_system_score_codex":0.0011535832,"about_ca_system_score_gemma":0.0009039165,"threshold_uncertainty_score":0.04430425},"labels":[],"label_agreement":null},{"id":"W2053831110","doi":"10.1088/0004-637x/794/1/23","title":"RAPIDLY EVOLVING AND LUMINOUS TRANSIENTS FROM PAN-STARRS1","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":354,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Australian Research Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Queen's University; Space Telescope Science Institute; University of Arizona; University of Edinburgh; Eötvös Loránd Tudományegyetem; European Commission; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; David and Lucile Packard Foundation; Jenny ja Antti Wihurin Rahasto; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Supernova; Blanketing; Physics; Redshift; Ejecta; Luminosity; Galaxy; Astronomy; Spectral line; Envelope (radar); Stars","score_opus":0.007116575384671947,"score_gpt":0.2055505242778436,"score_spread":0.19843394889317165,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053831110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99216604,0.001886955,0.0010482628,0.00010869969,0.00006248304,0.000045247565,0.0011673509,0.00009391971,0.0034209588],"genre_scores_gemma":[0.98995984,0.0014140308,0.0014883045,0.00019842204,0.0001133668,0.000020285346,0.005000194,0.000056283898,0.0017493335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973243,0.00001603009,0.000035203648,0.00008756536,0.00007366897,0.00005514773],"domain_scores_gemma":[0.9995289,0.00004199551,0.00014364855,0.00006978567,0.00009044805,0.00012519013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035525806,0.00041439908,0.00056164444,0.0014981854,0.0007999006,0.0015250978,0.0003868487,0.0005551147,0.0025285303],"category_scores_gemma":[0.000952532,0.00020739646,0.00038089318,0.0013506867,0.00031402122,0.0004969467,0.0010115819,0.0006412544,0.0014727622],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001303024,0.0002194069,0.7623613,0.0002974461,0.00016449044,0.0144118015,0.0016017966,0.00018348047,0.14995195,0.00050596567,0.001658612,0.06734082],"study_design_scores_gemma":[0.000017289838,0.00033301493,0.95734006,0.00005546368,0.000057989448,0.027605409,0.00050989416,0.00019173081,0.0044739894,0.00027656407,0.009116494,0.000022078048],"about_ca_topic_score_codex":0.0019493353,"about_ca_topic_score_gemma":0.002577353,"teacher_disagreement_score":0.0025285303,"about_ca_system_score_codex":0.0002353287,"about_ca_system_score_gemma":0.00017009916,"threshold_uncertainty_score":0.008458734},"labels":[],"label_agreement":null},{"id":"W2053947411","doi":"10.1086/521326","title":"SN 1993J VLBI. IV. A Geometric Distance to M81 with the Expanding Shock Front Method","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Shock (circulatory); Physics; Breakout; Supernova; Very-long-baseline interferometry; Astrophysics; Shock tube; Shock wave; Mechanics","score_opus":0.010799304329562002,"score_gpt":0.26298565678632574,"score_spread":0.25218635245676374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2053947411","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8894566,0.0013528494,0.050492946,0.00021945252,0.00009338783,0.00013836013,0.018462762,0.0014594055,0.038324274],"genre_scores_gemma":[0.92388266,0.00020807229,0.05135232,0.00006471809,0.00005485842,0.00009671647,0.019859483,0.00013405849,0.0043471023],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993988,0.000075872325,0.000030976465,0.00022738712,0.00019109188,0.00007580145],"domain_scores_gemma":[0.99891615,0.00013326014,0.0004297831,0.00017797839,0.0002560048,0.000086902524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007857385,0.0005546422,0.00031722075,0.0033920812,0.000339416,0.00081035215,0.0006477818,0.0004444325,0.002773883],"category_scores_gemma":[0.0022342487,0.00020596676,0.00041401488,0.0016972455,0.00019882584,0.00032958825,0.0010211077,0.00038480075,0.0017440552],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044913337,0.000066645436,0.8427587,0.00016608792,0.00046279727,0.00024305322,0.00023680711,0.01967187,0.013579123,0.009121514,0.008087408,0.10515693],"study_design_scores_gemma":[0.000032146272,0.00009463925,0.9488797,0.000026161513,0.0000835617,0.0004587543,0.000115121424,0.027754309,0.0070341425,0.001677828,0.013807663,0.000035950205],"about_ca_topic_score_codex":0.0137660215,"about_ca_topic_score_gemma":0.01595198,"teacher_disagreement_score":0.0137660215,"about_ca_system_score_codex":0.0010395587,"about_ca_system_score_gemma":0.00030396925,"threshold_uncertainty_score":0.027371764},"labels":[],"label_agreement":null},{"id":"W2054060101","doi":"10.1088/0004-637x/710/2/1710","title":"TIMING BEHAVIOR OF THE MAGNETICALLY ACTIVE ROTATION-POWERED PULSAR IN THE SUPERNOVA REMNANT KESTEVEN 75","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Glitch; Magnetar; Pulsar; Physics; Astrophysics; Rotation (mathematics); Astronomy; Supernova; Supernova remnant; Noise (video); Neutron star; Detector; Optics","score_opus":0.013389018295611522,"score_gpt":0.3118693524944914,"score_spread":0.29848033419887987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054060101","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99946874,0.000056155804,0.000058972582,0.000004789394,0.0000019457489,0.0000012583204,0.000043924534,0.00000935193,0.0003548447],"genre_scores_gemma":[0.9994836,0.000026794167,0.000107302774,0.0000048503507,0.0000028919217,0.000001812831,0.00018828093,0.0000035143416,0.00018098859],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999714,0.000002904358,0.0000026723915,0.00000769586,0.000008166661,0.000007121635],"domain_scores_gemma":[0.9998716,0.00001420847,0.00005733773,0.000012331107,0.000015256537,0.000029225179],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000097686425,0.00012631307,0.00019314907,0.00054368336,0.00016366573,0.0002479335,0.0001651355,0.00016279165,0.00050066266],"category_scores_gemma":[0.0003575256,0.00009300357,0.00008999004,0.00022275145,0.00017529722,0.00010326053,0.00031413953,0.00016097564,0.00017717356],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012164875,0.00016050691,0.61756957,0.00009723397,0.00017983002,0.005023664,0.00065352337,0.00384885,0.3396971,0.00084176037,0.0007735363,0.029937971],"study_design_scores_gemma":[0.000025982257,0.00034336947,0.98571044,0.0000068827935,0.00002657318,0.0010523271,0.00007487954,0.0029915136,0.008141775,0.00013641137,0.0014750311,0.000014720827],"about_ca_topic_score_codex":0.0012288474,"about_ca_topic_score_gemma":0.0020368835,"teacher_disagreement_score":0.0012288474,"about_ca_system_score_codex":0.00017732414,"about_ca_system_score_gemma":0.00006571627,"threshold_uncertainty_score":0.0024434328},"labels":[],"label_agreement":null},{"id":"W2054134963","doi":"10.1088/0004-637x/801/1/33","title":"STAR FORMATION IN DISK GALAXIES. III. DOES STELLAR FEEDBACK RESULT IN CLOUD DEATH?","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Star formation; Milky Way; Galaxy; Supernova; Astronomy; Molecular cloud; Gravitation; Stars","score_opus":0.017804916661179004,"score_gpt":0.24583161405293127,"score_spread":0.22802669739175227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054134963","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978752,0.0001176787,0.00039596108,0.000106608684,0.0000061797746,0.0000075505764,0.00008935532,0.0000118279,0.001389644],"genre_scores_gemma":[0.9995034,0.000035096502,0.000109382796,0.000019614827,0.0000019261756,0.0000020207874,0.000046374375,0.000005107926,0.00027713372],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990416,0.000024920786,0.0000044934595,0.000016154661,0.000012907236,0.000037408994],"domain_scores_gemma":[0.99954283,0.00014923938,0.00009423484,0.000034649973,0.000043230964,0.00013584874],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032031597,0.00029447494,0.0003769975,0.00019686247,0.0003745099,0.00054879166,0.0005100488,0.00058863993,0.0016175498],"category_scores_gemma":[0.0016648998,0.00015469019,0.0004346651,0.00017040207,0.0005711834,0.0005429638,0.0004247591,0.0003221704,0.00020354376],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091590855,0.00026991195,0.40203112,0.00016481709,0.0002516463,0.0010656676,0.00032105882,0.5518208,0.024165252,0.009660237,0.001063318,0.008270281],"study_design_scores_gemma":[0.00046018575,0.00055266364,0.15979381,0.00003370945,0.00012908531,0.00031061756,0.0006714399,0.8191387,0.008769592,0.008583729,0.0015219384,0.00003446852],"about_ca_topic_score_codex":0.012910843,"about_ca_topic_score_gemma":0.011196524,"teacher_disagreement_score":0.012910843,"about_ca_system_score_codex":0.00080430356,"about_ca_system_score_gemma":0.00033381872,"threshold_uncertainty_score":0.025671363},"labels":[],"label_agreement":null},{"id":"W2054152824","doi":"10.1088/0004-637x/796/2/109","title":"SEARCHES FOR EXTENDED AND POINT-LIKE NEUTRINO SOURCES WITH FOUR YEARS OF ICECUBE DATA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":199,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; U.S. Department of Energy; University of Wisconsin-Madison; Vetenskapsrådet; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; Vlaamse regering; University of Oxford; Compute Canada; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Neutrino; Neutrino astronomy; Astronomy; Astroparticle physics; Astrophysics; Point (geometry); Neutrino detector; Particle physics; Neutrino oscillation","score_opus":0.022333216381142485,"score_gpt":0.24123280043964462,"score_spread":0.21889958405850213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054152824","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9530877,0.0013037259,0.003735802,0.00021261927,0.000044450102,0.000061498875,0.036744498,0.0005502179,0.0042595514],"genre_scores_gemma":[0.7385704,0.001150824,0.0153091075,0.00013201643,0.00009332949,0.00019370233,0.24221691,0.00021380451,0.0021199598],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986865,0.0003205958,0.0000976381,0.00033772588,0.00031926096,0.00023827428],"domain_scores_gemma":[0.9963271,0.00158068,0.000605823,0.00067143474,0.00046207986,0.0003528915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002317913,0.00089890836,0.0009310898,0.002982507,0.0006048866,0.0017238172,0.0008745319,0.0007204473,0.0018855571],"category_scores_gemma":[0.0044643367,0.0003540998,0.0012800517,0.0033133375,0.00040122814,0.0010651321,0.0017782527,0.000536689,0.00069272623],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031017303,0.0005776168,0.8326759,0.0006751408,0.0027995047,0.0009931587,0.0005463605,0.053097796,0.015763735,0.0023809215,0.01601792,0.07137025],"study_design_scores_gemma":[0.0004286485,0.0007451942,0.8351406,0.00022253278,0.0012271778,0.0015730977,0.0007235617,0.059686333,0.022510478,0.0042693443,0.07323519,0.00023782907],"about_ca_topic_score_codex":0.0069691627,"about_ca_topic_score_gemma":0.01111461,"teacher_disagreement_score":0.0069691627,"about_ca_system_score_codex":0.0006077147,"about_ca_system_score_gemma":0.00093386613,"threshold_uncertainty_score":0.013857186},"labels":[],"label_agreement":null},{"id":"W2054269321","doi":"10.1086/522875","title":"Multiplicity among Young Brown Dwarfs and Very Low Mass Stars","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Multiplicity (mathematics); Low Mass; Stars; Binary number; Binary star; Star formation","score_opus":0.007382539720727859,"score_gpt":0.21239349528881396,"score_spread":0.2050109555680861,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054269321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996038,0.00007788425,0.00007960359,0.000004634492,5.548583e-7,0.0000013893946,0.000058824164,0.000003960108,0.00016938506],"genre_scores_gemma":[0.99909735,0.000070450966,0.00023488516,0.0000073562896,0.0000054326365,0.000002362612,0.00031401592,0.0000024963626,0.00026559076],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973387,0.000031706015,0.000020789466,0.000081972445,0.00006417894,0.000067481575],"domain_scores_gemma":[0.99892837,0.00014544775,0.0004498494,0.000070286995,0.00007725525,0.00032868554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003549855,0.00020776679,0.00029336585,0.002218693,0.00046465086,0.000544773,0.00031099186,0.00023507865,0.00066745566],"category_scores_gemma":[0.0008287201,0.00021248379,0.0001220798,0.0008717855,0.0004232319,0.00047732846,0.00065626996,0.00015685413,0.00034576096],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003755126,0.000010589466,0.99509454,0.000004982238,0.0000071942095,0.0000686059,0.0001653135,0.00002068788,0.0021574942,0.000021365682,0.000030673797,0.0023808768],"study_design_scores_gemma":[0.000001319392,0.00003371254,0.9988164,0.0000014729103,0.0000044609687,0.0003787382,0.00011939612,0.00006810906,0.00038213664,0.000023507373,0.00016865644,0.0000022088282],"about_ca_topic_score_codex":0.0037051996,"about_ca_topic_score_gemma":0.0058246823,"teacher_disagreement_score":0.0037051996,"about_ca_system_score_codex":0.0002901108,"about_ca_system_score_gemma":0.00016044512,"threshold_uncertainty_score":0.0073672533},"labels":[],"label_agreement":null},{"id":"W2054278703","doi":"10.1086/324782","title":"The Supernova Remnant CTB 104A: Magnetic Field Structure and Interaction with the Environment","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Supernova remnant; Physics; Astrophysics; Magnetic field; Spectral index; Velocity gradient; Supernova; Spectral line; Astronomy","score_opus":0.004860892824362292,"score_gpt":0.17761490753770637,"score_spread":0.17275401471334406,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054278703","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991416,0.000119522614,0.000085694344,0.000015105336,0.0000014334973,0.0000019728398,0.00011646574,0.00001642868,0.000501818],"genre_scores_gemma":[0.9988199,0.0000680919,0.00027248188,0.000009002048,0.0000053285294,0.0000023248801,0.00058464933,0.000007273747,0.0002308619],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996734,0.0000026257508,0.0000015349733,0.000009431375,0.000009037323,0.000009960567],"domain_scores_gemma":[0.9998672,0.000010506249,0.000040660416,0.000010794548,0.000014789941,0.000056093606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000044418266,0.0002213537,0.00018863443,0.0006322508,0.00024824688,0.0003127118,0.00026090484,0.00021656162,0.0010032391],"category_scores_gemma":[0.00018947625,0.000110110785,0.000118167845,0.00044671423,0.00028761485,0.00012168464,0.00033373185,0.00024300313,0.00024632795],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009533496,0.00014043601,0.38524395,0.000112282076,0.00012509603,0.0036952707,0.00031940127,0.0027512389,0.5896397,0.00030462153,0.0006852393,0.016029302],"study_design_scores_gemma":[0.000012590191,0.000085922075,0.9925552,0.000004875831,0.000017381706,0.0011010492,0.00007046388,0.0012870312,0.004061659,0.00005438234,0.000738383,0.000011019484],"about_ca_topic_score_codex":0.0072945585,"about_ca_topic_score_gemma":0.008509633,"teacher_disagreement_score":0.0072945585,"about_ca_system_score_codex":0.00026584626,"about_ca_system_score_gemma":0.00008381074,"threshold_uncertainty_score":0.014504194},"labels":[],"label_agreement":null},{"id":"W2054306542","doi":"10.1086/525038","title":"VLT Spectroscopy of Globular Clusters in Low Surface Brightness Dwarf Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Surface brightness; Spectroscopy; Dwarf galaxy; Galaxy; Dwarf spheroidal galaxy; Brightness; Astronomical spectroscopy","score_opus":0.006768322267860431,"score_gpt":0.21001840668320948,"score_spread":0.20325008441534906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054306542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98822975,0.0006995905,0.0009247272,0.0007532914,0.00020944315,0.000027983257,0.0014009515,0.00029639326,0.007457802],"genre_scores_gemma":[0.98994195,0.0002160667,0.0007439564,0.00018347295,0.000151801,0.0000126187,0.0016146553,0.00006483973,0.0070706536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997055,0.000022713015,0.000010863455,0.000080120095,0.00010261833,0.00007817579],"domain_scores_gemma":[0.99895203,0.00014249881,0.00011965607,0.00009481438,0.00035855983,0.00033234656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006424265,0.00023139412,0.00044039084,0.001730774,0.00074340566,0.0007942917,0.00050945557,0.0007762993,0.006447241],"category_scores_gemma":[0.0013679008,0.00022040894,0.00020597677,0.0008123508,0.00025696994,0.00033730266,0.00052017206,0.00022438064,0.0021180192],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018987543,0.00026071907,0.66168654,0.0003343615,0.00020318264,0.0019485668,0.0007296248,0.0008082475,0.24539742,0.0010784329,0.033173457,0.052480727],"study_design_scores_gemma":[0.00010217876,0.00018080717,0.97480893,0.00003309507,0.00007741967,0.0006539213,0.0003777308,0.0021186785,0.013613386,0.000547888,0.0074629677,0.000022941631],"about_ca_topic_score_codex":0.0024365042,"about_ca_topic_score_gemma":0.005381961,"teacher_disagreement_score":0.006447241,"about_ca_system_score_codex":0.0004699256,"about_ca_system_score_gemma":0.00029204143,"threshold_uncertainty_score":0.021568239},"labels":[],"label_agreement":null},{"id":"W2054353864","doi":"10.1086/501002","title":"Detecting Interstellar Alkanes","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Spectral line; Astrophysics; Absorption (acoustics); Interstellar medium; Alkane; Absorption spectroscopy; Molecule; Molecular cloud; Astrochemistry; Interstellar cloud; Infrared; Astronomy; Galaxy; Hydrocarbon; Stars; Optics; Chemistry","score_opus":0.007359872148075485,"score_gpt":0.21839770809267803,"score_spread":0.21103783594460254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054353864","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99057347,0.00055912096,0.0027448134,0.000026040363,0.000010535365,0.000018771363,0.00039012838,0.00010281782,0.005574351],"genre_scores_gemma":[0.99012566,0.00030241197,0.0068719615,0.00006029287,0.000013884045,0.00002288564,0.0006094654,0.000014751707,0.0019786134],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991834,0.0000058517226,0.0000016038261,0.000029406092,0.000022601069,0.00002218613],"domain_scores_gemma":[0.9998609,0.000028552853,0.000028420685,0.000013342732,0.000030102854,0.000038688453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000113718605,0.00017219319,0.000110730856,0.00058228476,0.00025048034,0.00020332653,0.00026539067,0.00035932707,0.0016675196],"category_scores_gemma":[0.00022292335,0.00011388626,0.00008527036,0.00030254677,0.00010477092,0.00025302148,0.00036125103,0.00022630917,0.00036959507],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015083345,0.000036495465,0.06278734,0.00008082353,0.000028011385,0.00014689562,0.00011606122,0.00018519013,0.91535133,0.00029860265,0.00027410284,0.02054435],"study_design_scores_gemma":[0.000026507563,0.00023814166,0.55118114,0.000028322462,0.00007498715,0.00081302074,0.00023560369,0.0023123738,0.43832758,0.0004668585,0.006278818,0.000016598835],"about_ca_topic_score_codex":0.0006956689,"about_ca_topic_score_gemma":0.0020983156,"teacher_disagreement_score":0.0016675196,"about_ca_system_score_codex":0.00016189861,"about_ca_system_score_gemma":0.00008004067,"threshold_uncertainty_score":0.0055784583},"labels":[],"label_agreement":null},{"id":"W2054430631","doi":"10.1088/0004-637x/786/2/153","title":"ASYMMETRIC ORBITAL DISTRIBUTION NEAR MEAN MOTION RESONANCE: APPLICATION TO PLANETS OBSERVED BY<i>KEPLER</i>AND RADIAL VELOCITIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Mean motion; Radial velocity; Eccentricity (behavior); Orbital period; Orbital elements; Orbit (dynamics); Orbital inclination; Orbital speed; Orbital eccentricity","score_opus":0.00899175720344645,"score_gpt":0.20338309850272784,"score_spread":0.1943913412992814,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054430631","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98661894,0.00017852617,0.011088453,0.000061649946,0.000004689899,0.000008008973,0.00007472517,0.000052436015,0.0019125072],"genre_scores_gemma":[0.9984326,0.000058864323,0.0013628985,0.0000032846071,0.000003845944,0.0000019510417,0.000019473713,0.000008848046,0.00010827158],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99991715,0.000021653614,0.000004487188,0.000022700018,0.000014860908,0.000019109173],"domain_scores_gemma":[0.99937564,0.00029444962,0.00017341856,0.000068207264,0.000040209106,0.000048013844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023354855,0.00015244704,0.00022117648,0.00074388506,0.00034432427,0.0005024361,0.0004378713,0.00031408592,0.00053890527],"category_scores_gemma":[0.0022597825,0.00018905489,0.00027349967,0.0006464451,0.0003940236,0.000513957,0.000461971,0.00023493907,0.00009312941],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002467257,0.00007866711,0.28909346,0.00014449225,0.0000740319,0.0027357857,0.0009402797,0.5840394,0.053641606,0.033678275,0.0007340008,0.034593303],"study_design_scores_gemma":[0.000011117171,0.00002444802,0.047290426,0.000006726412,0.000015947104,0.0006078027,0.00012749943,0.9446264,0.0023346427,0.0042980653,0.00063820306,0.000018704819],"about_ca_topic_score_codex":0.004922368,"about_ca_topic_score_gemma":0.0023419275,"teacher_disagreement_score":0.004922368,"about_ca_system_score_codex":0.00054705964,"about_ca_system_score_gemma":0.00021715442,"threshold_uncertainty_score":0.00978744},"labels":[],"label_agreement":null},{"id":"W2054498796","doi":"10.1088/0004-637x/762/1/33","title":"INTERACTING COSMIC RAYS WITH MOLECULAR CLOUDS: A BREMSSTRAHLUNG ORIGIN OF DIFFUSE HIGH-ENERGY EMISSION FROM THE INNER 2°×1° OF THE GALACTIC CENTER","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":146,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Bremsstrahlung; Astrophysics; Galactic Center; Population; Cosmic ray; Molecular cloud; Electron; Ionization; Fermi Gamma-ray Space Telescope; Synchrotron radiation; Astronomy; Galaxy; Ion; Nuclear physics; Stars","score_opus":0.006785798093629098,"score_gpt":0.2122022907364748,"score_spread":0.20541649264284573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054498796","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980952,0.00024463766,0.00072339765,0.000024836636,0.0000013772922,0.0000056018575,0.000058183006,0.000026361144,0.0008204286],"genre_scores_gemma":[0.99927443,0.00008453865,0.00043212203,0.000010652187,0.0000030048277,0.0000019992528,0.00008174465,0.0000053933513,0.00010616595],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999951,0.000005261604,0.00000252262,0.000014566184,0.000012209516,0.000014543531],"domain_scores_gemma":[0.9998746,0.000016982996,0.000053647065,0.000013268909,0.000009303687,0.00003222871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008421113,0.0003747751,0.0002489205,0.00030604578,0.0003201667,0.000773609,0.0003432581,0.0002802374,0.0010247808],"category_scores_gemma":[0.00023473689,0.0002167928,0.00029484494,0.00041913538,0.00025158946,0.00031057588,0.0003438742,0.0002278088,0.00018241582],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024644143,0.000086397355,0.914603,0.000056517856,0.000106397725,0.0008262661,0.00020531948,0.004767254,0.06887837,0.002323386,0.00017507459,0.007725482],"study_design_scores_gemma":[0.00004787144,0.00011452186,0.9682045,0.000026806081,0.00009307561,0.000624377,0.00015616007,0.01962239,0.00911804,0.000981109,0.0009965282,0.000014545387],"about_ca_topic_score_codex":0.0048581087,"about_ca_topic_score_gemma":0.0064034206,"teacher_disagreement_score":0.0048581087,"about_ca_system_score_codex":0.0005017443,"about_ca_system_score_gemma":0.00018743107,"threshold_uncertainty_score":0.009659648},"labels":[],"label_agreement":null},{"id":"W2054522960","doi":"10.1088/0004-637x/787/2/99","title":"DEGREE OF POLARIZATION AND SOURCE COUNTS OF FAINT RADIO SOURCES FROM STACKING POLARIZED INTENSITY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Calgary","funders":"","keywords":"Stacking; Polarization (electrochemistry); Physics; Sky; Linear polarization; Astrophysics; Monte Carlo method; Quartile; Computational physics; Optics; Nuclear magnetic resonance; Statistics; Chemistry; Mathematics","score_opus":0.011419996414828599,"score_gpt":0.205002162955972,"score_spread":0.1935821665411434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054522960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98857003,0.000076505734,0.009212209,0.00001460072,0.0000047155686,0.000005782133,0.0005796588,0.00013153524,0.0014049928],"genre_scores_gemma":[0.9948832,0.000050624425,0.0031628113,0.0000085850315,0.000011381782,0.0000065243125,0.0017007987,0.00003067553,0.00014543347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99952185,0.00009809167,0.000025629404,0.000118225034,0.00015069933,0.00008551775],"domain_scores_gemma":[0.996274,0.0013283257,0.0010617661,0.0005967794,0.00051076995,0.00022837863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000926038,0.00038990538,0.00030382324,0.0019220219,0.00030346224,0.0010743298,0.00028330178,0.00034202565,0.0012989059],"category_scores_gemma":[0.0051764506,0.00028826052,0.00039059232,0.0016201255,0.00052428595,0.0007030398,0.00084357744,0.00042267062,0.00033086704],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027778963,0.000039513412,0.9199526,0.000048758273,0.00013826699,0.00018537615,0.00030227777,0.023454059,0.02292484,0.0020765807,0.00041174472,0.030188262],"study_design_scores_gemma":[0.0000052342225,0.00005219948,0.94976485,0.000015986168,0.000090464666,0.0003912946,0.00014578711,0.03468601,0.01120871,0.0026604705,0.00093844667,0.000040518924],"about_ca_topic_score_codex":0.0011792437,"about_ca_topic_score_gemma":0.0011411111,"teacher_disagreement_score":0.0019220219,"about_ca_system_score_codex":0.00025465267,"about_ca_system_score_gemma":0.00016197258,"threshold_uncertainty_score":0.0048974156},"labels":[],"label_agreement":null},{"id":"W2054706807","doi":"10.1086/431731","title":"Latitudinal Shear Instabilities during Type I X‐Ray Bursts","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Differential rotation; Equator; Astrophysics; Neutron star; Instability; Amplitude; Vorticity; Wavenumber; Mechanics; Vortex; Optics; Astronomy; Stars","score_opus":0.014422591963652689,"score_gpt":0.2350090724593772,"score_spread":0.2205864804957245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054706807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994773,0.000062028004,0.00020384646,0.000008931575,0.0000015929568,0.0000023664988,0.000024576022,0.000011439304,0.0002079794],"genre_scores_gemma":[0.99967587,0.00004975562,0.000112147725,0.00000405437,0.0000038828157,0.000002941925,0.000057598918,0.000003530054,0.00009021675],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999467,0.0000067369924,0.000007773148,0.000013309816,0.000012931244,0.000012586539],"domain_scores_gemma":[0.9996393,0.00005073418,0.00020586829,0.000022467386,0.00003293217,0.00004874845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014752288,0.00024052979,0.00019718746,0.00040571415,0.0003134646,0.0005110024,0.00018731171,0.0002893622,0.00033685451],"category_scores_gemma":[0.0006076646,0.00020056806,0.00017227793,0.00023312675,0.0003661661,0.00023296943,0.0004218754,0.00021405442,0.000096098745],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009434888,0.00008283254,0.539936,0.000101059624,0.00012433439,0.00091636257,0.0010169089,0.015894156,0.4280231,0.0017803406,0.00033499958,0.010846338],"study_design_scores_gemma":[0.00011579902,0.0005222561,0.8796322,0.000022288417,0.000113844995,0.0007160287,0.0004183483,0.070777416,0.04593011,0.0007707385,0.0009309156,0.000050024795],"about_ca_topic_score_codex":0.0015383799,"about_ca_topic_score_gemma":0.0011560835,"teacher_disagreement_score":0.0015383799,"about_ca_system_score_codex":0.00034155822,"about_ca_system_score_gemma":0.000096022166,"threshold_uncertainty_score":0.0030589104},"labels":[],"label_agreement":null},{"id":"W2054732781","doi":"10.1086/521424","title":"Stromgren Photometry of Galactic Globular Clusters. I. New Calibrations of the Metallicity Index","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Metallicity; Globular cluster; Photometry (optics); Astrophysics; Physics; Stars; Red-giant branch; Astronomy","score_opus":0.01183553184328881,"score_gpt":0.23854024699588047,"score_spread":0.22670471515259166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054732781","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8679303,0.024167089,0.018492414,0.0033014163,0.0014271771,0.0001673212,0.020216657,0.00215287,0.062144686],"genre_scores_gemma":[0.94688845,0.008041603,0.010889323,0.00038924717,0.0011032793,0.000045396635,0.0088325795,0.0002630757,0.02354698],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99939823,0.00008212001,0.000056489956,0.00012433891,0.0002968504,0.00004196132],"domain_scores_gemma":[0.9970024,0.00041221015,0.00038892974,0.00049881544,0.0014418227,0.00025585474],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019894843,0.00034761828,0.00040961689,0.0026871737,0.00031412425,0.0009146542,0.0006975766,0.00055041746,0.0061612],"category_scores_gemma":[0.0033556023,0.00022750536,0.00022140394,0.0020984635,0.00050300965,0.0010719824,0.00064698374,0.0004888887,0.0044610915],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000844246,0.00011833263,0.5941022,0.0010567916,0.00021333458,0.0003286685,0.0008149144,0.0013232842,0.041070238,0.0057980423,0.044632893,0.309697],"study_design_scores_gemma":[0.000079616184,0.000092000366,0.9377217,0.00018553133,0.00011927574,0.00036372727,0.00026912446,0.0014575875,0.010100757,0.0017959247,0.047766812,0.00004789061],"about_ca_topic_score_codex":0.0044724904,"about_ca_topic_score_gemma":0.015260706,"teacher_disagreement_score":0.0061612,"about_ca_system_score_codex":0.0009565964,"about_ca_system_score_gemma":0.00042608276,"threshold_uncertainty_score":0.020611286},"labels":[],"label_agreement":null},{"id":"W2054753318","doi":"10.1088/0004-637x/783/1/7","title":"THE MASSES OF LOCAL GROUP DWARF SPHEROIDAL GALAXIES: THE DEATH OF THE UNIVERSAL MASS PROFILE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Dalhousie University","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Andromeda; Milky Way; Local Group; Dark matter; Galaxy; Sigma; Halo; Stellar kinematics; Dwarf galaxy","score_opus":0.005408418321727529,"score_gpt":0.19256743840818508,"score_spread":0.18715902008645754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054753318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99836785,0.00011113246,0.00060042844,0.00003828509,0.0000013938095,0.0000013114624,0.000072809366,0.000014619186,0.00079211366],"genre_scores_gemma":[0.9997346,0.0000203034,0.00011369895,0.0000043454606,0.000002565375,6.937126e-7,0.000066695684,0.0000035347825,0.000053552714],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999757,0.00006456842,0.00001173923,0.0000750109,0.000045320383,0.000046481127],"domain_scores_gemma":[0.99677426,0.0008649809,0.0009725493,0.0006971015,0.0002762252,0.00041479984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011155428,0.00022337738,0.0002833523,0.0010582806,0.00035912378,0.00072388106,0.0005575005,0.00022612196,0.0009459092],"category_scores_gemma":[0.004708397,0.00010602005,0.00022273192,0.0005720341,0.0010098919,0.0007832932,0.0009616512,0.00029025742,0.00030894656],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026645002,0.000012118366,0.9755754,0.000018949146,0.000051272593,0.00016021288,0.00070377963,0.0014620676,0.0035241274,0.0042332886,0.00020976302,0.013782472],"study_design_scores_gemma":[0.000017726241,0.000114265276,0.97740674,0.000025846755,0.000046296485,0.00040654553,0.001024992,0.0102068335,0.0030421962,0.006741067,0.00094899465,0.000018460942],"about_ca_topic_score_codex":0.0031945459,"about_ca_topic_score_gemma":0.0023626115,"teacher_disagreement_score":0.0031945459,"about_ca_system_score_codex":0.000423152,"about_ca_system_score_gemma":0.00015125539,"threshold_uncertainty_score":0.006351888},"labels":[],"label_agreement":null},{"id":"W2054829972","doi":"10.1088/0004-637x/740/2/108","title":"CFBDSIR J1458+1013B: A VERY COLD (&gt;T10) BROWN DWARF IN A BINARY SYSTEM, ,","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Brown dwarf; Photometry (optics); Stellar classification; Luminosity; Surface gravity; Parallax; Effective temperature; Low Mass; Starspot","score_opus":0.016645207593757278,"score_gpt":0.20726293322254968,"score_spread":0.1906177256287924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054829972","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9867251,0.0004108179,0.00044876136,0.0011078748,0.00024681122,0.000031601387,0.00082979305,0.00011425172,0.010084997],"genre_scores_gemma":[0.993389,0.000053139014,0.00043732623,0.0006909928,0.00014702365,0.000007930746,0.0008130339,0.000040474097,0.004420865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981695,0.000010773478,0.000012177171,0.00006217507,0.00003855012,0.00005944941],"domain_scores_gemma":[0.9992354,0.000059639693,0.00011590513,0.000030361121,0.000045542944,0.0005132281],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039807532,0.0007380599,0.00091545976,0.0011642128,0.0024326215,0.001205948,0.00084485376,0.0024795672,0.004975622],"category_scores_gemma":[0.0004414208,0.0004028587,0.00040596543,0.00075883634,0.00093664724,0.00046723694,0.00086600287,0.0013286036,0.0024596024],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004497239,0.0013161383,0.42388684,0.00039755818,0.00020984115,0.17175114,0.0020345002,0.001148011,0.30410326,0.0048262686,0.041050717,0.044778477],"study_design_scores_gemma":[0.00052680576,0.0020575586,0.82311577,0.00006166156,0.0001419322,0.11780181,0.0014433735,0.0038167965,0.016180819,0.0025872265,0.032164007,0.000102136284],"about_ca_topic_score_codex":0.011369966,"about_ca_topic_score_gemma":0.016569765,"teacher_disagreement_score":0.011369966,"about_ca_system_score_codex":0.0012359757,"about_ca_system_score_gemma":0.000544296,"threshold_uncertainty_score":0.022607565},"labels":[],"label_agreement":null},{"id":"W2054836946","doi":"10.1088/0004-637x/722/2/1180","title":"GALAXY CLUSTERS SELECTED WITH THE SUNYAEV-ZEL'DOVICH EFFECT FROM 2008 SOUTH POLE TELESCOPE OBSERVATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":335,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; W. M. Keck Foundation; National Science Foundation","keywords":"Redshift; CMB cold spot; Cosmology; Galaxy cluster; Galaxy; South Pole Telescope; Sky; Cluster (spacecraft); Telescope","score_opus":0.0055602359422138705,"score_gpt":0.19173385272614435,"score_spread":0.1861736167839305,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054836946","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99692994,0.00009613446,0.00027694635,0.000021408234,0.0000031174782,0.000011032139,0.0014603521,0.000026438793,0.0011747386],"genre_scores_gemma":[0.9966768,0.00005010448,0.0003269526,0.000012286362,0.000007004672,0.000009765358,0.0026780749,0.000006855721,0.00023212243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997416,0.000024574034,0.000013499522,0.00009143362,0.00007231636,0.000056585457],"domain_scores_gemma":[0.9993144,0.00012049869,0.00026342436,0.00012558844,0.0000522247,0.00012394716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022318408,0.00018451766,0.00027086653,0.0013204217,0.00033754954,0.0004894249,0.0002725033,0.00014149726,0.001733099],"category_scores_gemma":[0.0009120831,0.00014736304,0.00014537963,0.00068798126,0.00027016498,0.00018671401,0.0007329496,0.00011194156,0.00025510392],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008148679,0.000014827158,0.98897105,0.000019719824,0.00003135717,0.0001365523,0.00012935161,0.0005398334,0.0025408065,0.00018568173,0.0011418696,0.0062073055],"study_design_scores_gemma":[0.000008436013,0.000010685783,0.99794966,0.0000025896913,0.000009036539,0.00009032124,0.0000312074,0.0005119131,0.0003258377,0.000042362077,0.0010154505,0.0000024736091],"about_ca_topic_score_codex":0.008923605,"about_ca_topic_score_gemma":0.02182792,"teacher_disagreement_score":0.008923605,"about_ca_system_score_codex":0.00035440308,"about_ca_system_score_gemma":0.00027233266,"threshold_uncertainty_score":0.01774329},"labels":[],"label_agreement":null},{"id":"W2054884156","doi":"10.1088/0004-637x/758/2/136","title":"HOT DISKS AND DELAYED BAR FORMATION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Galaxy; Bar (unit); Star formation; Galaxy formation and evolution; Stellar mass; Baryon; Cold dark matter; Dark matter; Interacting galaxy","score_opus":0.008858836974293582,"score_gpt":0.21629936667001773,"score_spread":0.20744052969572416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054884156","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990876,0.00021299456,0.00006530297,0.000027309568,0.0000018376325,0.0000013127459,0.00008986253,0.0000032325665,0.00051052973],"genre_scores_gemma":[0.999665,0.000047402296,0.000034793688,0.000009730638,0.000005913536,8.452766e-7,0.000077922006,7.159082e-7,0.0001575711],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998678,0.000020167592,0.000009307617,0.00003663401,0.000023065151,0.000042944794],"domain_scores_gemma":[0.996761,0.00041534237,0.0018528489,0.00018430952,0.00017057438,0.00061586715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027557035,0.00014333133,0.00014898814,0.00088883034,0.00029053207,0.0006254605,0.00036308158,0.00029140533,0.001976201],"category_scores_gemma":[0.0015285201,0.00014235513,0.00011324821,0.0004542843,0.00047212388,0.00031457408,0.00055477617,0.0003697567,0.00024619882],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012045389,0.000022090038,0.9955581,0.000012054887,0.000013707033,0.00015897822,0.00012398096,0.00003441573,0.0018711885,0.00010956308,0.000033286135,0.0019422474],"study_design_scores_gemma":[0.0000028824927,0.000036331476,0.99891055,0.0000029825876,0.0000098107375,0.00038188958,0.00007319651,0.00004887382,0.0002447033,0.000091216585,0.00019561332,0.0000018414731],"about_ca_topic_score_codex":0.0019439268,"about_ca_topic_score_gemma":0.0029052815,"teacher_disagreement_score":0.001976201,"about_ca_system_score_codex":0.00016302482,"about_ca_system_score_gemma":0.00011392178,"threshold_uncertainty_score":0.006611049},"labels":[],"label_agreement":null},{"id":"W2054913235","doi":"10.1088/0004-637x/760/1/26","title":"THE FREQUENCY OF DEBRIS DISKS AT WHITE DWARFS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Dwarf planet; Asteroid; Stars; Astrophysics; Photometry (optics); Planet; Astronomy; Metallicity; Debris; Accretion (finance); Infrared excess; Planetesimal; Black dwarf; Astrobiology","score_opus":0.012071939744492412,"score_gpt":0.22949313873180227,"score_spread":0.21742119898730985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054913235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942756,0.00006969354,0.00006813552,0.000007675788,9.1087713e-7,8.9741144e-7,0.00010271873,0.0000073688757,0.00031504646],"genre_scores_gemma":[0.9994598,0.000026711225,0.00005639213,0.0000039715187,0.0000032677485,0.0000010736991,0.00022701877,0.0000023336315,0.0002194093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997999,0.000018003851,0.000011792743,0.000067417335,0.000055006476,0.00004788334],"domain_scores_gemma":[0.99916327,0.00012551162,0.0003408953,0.000067583285,0.00012402878,0.00017877202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020947825,0.00012963146,0.00015806592,0.0018258056,0.00037046673,0.00051560986,0.00024683223,0.00021218842,0.0012647207],"category_scores_gemma":[0.0007873478,0.00009269236,0.00011111798,0.000575393,0.00029740843,0.00028572982,0.0005006954,0.000102659185,0.000397017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004701362,0.000007669648,0.9917,0.0000065031522,0.000009014974,0.00008509788,0.00029026542,0.000019441359,0.0036142531,0.000067129535,0.00006724283,0.0040863305],"study_design_scores_gemma":[0.0000014225649,0.000026901107,0.99792504,0.000002184242,0.0000050902245,0.00041428526,0.00016043734,0.00006315551,0.00096095924,0.000043309305,0.00039517862,0.0000019305282],"about_ca_topic_score_codex":0.0011712996,"about_ca_topic_score_gemma":0.0018776059,"teacher_disagreement_score":0.0018258056,"about_ca_system_score_codex":0.00015527199,"about_ca_system_score_gemma":0.00006840564,"threshold_uncertainty_score":0.0042309165},"labels":[],"label_agreement":null},{"id":"W2054929031","doi":"10.1086/591240","title":"The Regulation of Cooling and Star Formation in Luminous Galaxies by Active Galactic Nucleus Feedback and the Cooling‐Time/Entropy Threshold for the Onset of Star Formation","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":258,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Intracluster medium; Star formation; Supermassive black hole; Astronomy; Galaxy; Virgo Cluster; Galaxy cluster; Cooling flow","score_opus":0.008324180798371803,"score_gpt":0.20575088356581742,"score_spread":0.19742670276744562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054929031","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99979764,0.00003459428,0.00007030925,0.000002502915,1.731081e-7,8.2621807e-7,0.000019665018,0.0000035192766,0.00007079194],"genre_scores_gemma":[0.99989545,0.00001021771,0.000047378955,0.000001699175,8.000763e-7,8.4373727e-7,0.00002547607,8.4143346e-7,0.000017270635],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999062,0.000017003305,0.0000067362503,0.000025605563,0.000012557698,0.000031936124],"domain_scores_gemma":[0.9988167,0.0003623003,0.00054341677,0.00009652707,0.00006184293,0.000119191725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030066536,0.00014256475,0.00022029085,0.0007492158,0.00018173372,0.00055370724,0.00023577563,0.00019872672,0.0003768162],"category_scores_gemma":[0.001401348,0.00013559291,0.00012502882,0.00030155442,0.0005626399,0.00023558598,0.00032820826,0.00016109325,0.000074110365],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022747753,0.000032854983,0.94486797,0.000013373523,0.00002896358,0.00007712176,0.0002460003,0.0006707484,0.04998857,0.00027069045,0.000028106377,0.0035480373],"study_design_scores_gemma":[0.0000046924333,0.000040870545,0.9955636,0.0000011592522,0.0000084623925,0.00011344855,0.000050400136,0.0010059245,0.0030492158,0.00011538224,0.000043309792,0.0000033705692],"about_ca_topic_score_codex":0.0021087716,"about_ca_topic_score_gemma":0.002350531,"teacher_disagreement_score":0.0021087716,"about_ca_system_score_codex":0.00034395044,"about_ca_system_score_gemma":0.00012021566,"threshold_uncertainty_score":0.0041929483},"labels":[],"label_agreement":null},{"id":"W2054945010","doi":"10.1086/309208","title":"The H<scp>ii</scp>Region KR 140: Spontaneous Formation of a High‐Mass Star","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Nebula; Molecular cloud; Galactic plane; Star formation; Star (game theory); Orion Nebula; Emission nebula; Context (archaeology); Extinction (optical mineralogy); Stars; H II region; Astronomy; Geography","score_opus":0.006921727102880117,"score_gpt":0.20553384476033643,"score_spread":0.19861211765745632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054945010","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988147,0.00003191931,0.0001787666,0.0000048982724,5.1522994e-7,0.000004453208,0.00015050986,0.0000071677323,0.000807184],"genre_scores_gemma":[0.9990256,0.000023150355,0.0003706573,0.000010393754,0.0000012716143,0.0000023806533,0.00041171853,0.0000035961568,0.00015121159],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986565,0.0000066811167,0.000005730855,0.00003440993,0.00004952403,0.00003800599],"domain_scores_gemma":[0.999632,0.000037160436,0.00014552342,0.00005440214,0.000056276767,0.00007471433],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018897431,0.00012065194,0.00016649632,0.00038400458,0.00033520727,0.00038584965,0.00035150527,0.0001172392,0.0004918102],"category_scores_gemma":[0.00037784193,0.00012922603,0.00011286764,0.00047432183,0.00035457933,0.0001947576,0.00049223815,0.00015987137,0.00016048888],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023741175,0.00007119181,0.8781699,0.00005997399,0.00008262348,0.0011663147,0.000752949,0.0004887431,0.10607105,0.0007770269,0.00030949197,0.011813376],"study_design_scores_gemma":[0.0000064650408,0.00009048164,0.9887883,0.0000036553304,0.000015248026,0.0010932072,0.00017469474,0.0003769864,0.0076409956,0.00010040384,0.0017032027,0.0000063444413],"about_ca_topic_score_codex":0.022676956,"about_ca_topic_score_gemma":0.0386635,"teacher_disagreement_score":0.022676956,"about_ca_system_score_codex":0.00047282514,"about_ca_system_score_gemma":0.0004562944,"threshold_uncertainty_score":0.0450899},"labels":[],"label_agreement":null},{"id":"W2054953373","doi":"10.1086/322356","title":"The Metamorphosis of Tidally Stirred Dwarf Galaxies","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":379,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; McMaster University","funders":"","keywords":"Milky Way; Dwarf galaxy problem; Dwarf galaxy; Dark matter; Dwarf spheroidal galaxy; Surface brightness; Galaxy; Dark matter halo","score_opus":0.013533902514158345,"score_gpt":0.26373686976094485,"score_spread":0.2502029672467865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2054953373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974598,0.000031355496,0.0007223431,0.000051096482,0.000007445431,0.000009897194,0.000099555225,0.00006615586,0.0015522703],"genre_scores_gemma":[0.99853873,0.000025073623,0.00079706806,0.000021564556,0.0000036577444,0.000007736041,0.00018832515,0.000016550222,0.00040128283],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998894,0.000021488193,0.0000060865095,0.000024045446,0.000020720723,0.000038245667],"domain_scores_gemma":[0.99939954,0.0001693679,0.00010405914,0.000066849316,0.000053940345,0.0002062872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029461342,0.00034838248,0.00037153717,0.00044939472,0.0006672992,0.0008879505,0.00076248246,0.00077152404,0.001684237],"category_scores_gemma":[0.0018210238,0.00035058864,0.0005590274,0.00032060288,0.0009966096,0.00053589954,0.0008003032,0.00059633533,0.00018340189],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003047909,0.00018623003,0.056876406,0.000036500773,0.00012284753,0.0005538562,0.00031055676,0.92929226,0.0050944835,0.0033255687,0.00057117105,0.003325342],"study_design_scores_gemma":[0.000079776975,0.000093073526,0.01138064,0.000006980048,0.000020030919,0.00006144877,0.00009761466,0.986217,0.0006843384,0.0009378298,0.00040932166,0.00001193134],"about_ca_topic_score_codex":0.021038737,"about_ca_topic_score_gemma":0.015661223,"teacher_disagreement_score":0.021038737,"about_ca_system_score_codex":0.0010422767,"about_ca_system_score_gemma":0.0006580305,"threshold_uncertainty_score":0.041832566},"labels":[],"label_agreement":null},{"id":"W2055007187","doi":"10.1086/427258","title":"An Absence of Hot Jupiter Planets in 47 Tucanae: Results of a Wide‐Field Transit Search","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Hot Jupiter; Planet; Transit (satellite); Exoplanet; Gas giant; Globular cluster; Orbital period; Jupiter (rocket family)","score_opus":0.01241194249682591,"score_gpt":0.24867819283893236,"score_spread":0.23626625034210644,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055007187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989876,0.00010935064,0.00003839217,0.000016546772,0.0000018438153,0.000004054667,0.0004073968,0.000007182242,0.0004276587],"genre_scores_gemma":[0.9974974,0.00012311315,0.00011492131,0.000018225675,0.0000069239695,0.000003071983,0.0019435807,0.0000048578877,0.00028802713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997867,0.000010453255,0.000007413782,0.000044709337,0.00004628239,0.00010451286],"domain_scores_gemma":[0.99916124,0.00012114132,0.00022433985,0.00008356619,0.00016617504,0.00024364637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002713592,0.00028865846,0.00039520598,0.0016027183,0.0012097084,0.00083595887,0.0004656958,0.00041388976,0.0012678608],"category_scores_gemma":[0.00082841143,0.00009718211,0.00017960365,0.0013687166,0.00058826973,0.00024988115,0.0006959225,0.00026937664,0.00020348401],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051922014,0.00008889505,0.9661338,0.000050508286,0.00013025408,0.0008732166,0.0006612763,0.00052277424,0.014470281,0.00018343997,0.00074354437,0.015622718],"study_design_scores_gemma":[0.000017871615,0.00008125274,0.9938791,0.000008468757,0.000085974665,0.00045017374,0.00077658193,0.00047131308,0.002233508,0.000046354297,0.0019403526,0.000008986909],"about_ca_topic_score_codex":0.12227179,"about_ca_topic_score_gemma":0.17125551,"teacher_disagreement_score":0.12227179,"about_ca_system_score_codex":0.00078952324,"about_ca_system_score_gemma":0.0013281216,"threshold_uncertainty_score":0.24312013},"labels":[],"label_agreement":null},{"id":"W2055015929","doi":"10.1088/0004-637x/749/2/126","title":"EVIDENCE FOR TYPE Ia SUPERNOVA DIVERSITY FROM ULTRAVIOLET OBSERVATIONS WITH THE<i>HUBBLE SPACE TELESCOPE</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Quest University Canada; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; National Natural Science Foundation of China; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; U.S. Department of Energy; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Photometry (optics); Supernova; Ultraviolet; Light curve; Metallicity; Spectroscopy; Hubble Deep Field South; Spectral line; Hubble space telescope; Astronomy; Stars; Hubble Deep Field; Optics","score_opus":0.06986909120254584,"score_gpt":0.2794258619171012,"score_spread":0.2095567707145554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055015929","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99887186,0.00015864342,0.00016780599,0.000010194642,0.0000025123272,0.0000024607778,0.00021806109,0.000011699143,0.0005567262],"genre_scores_gemma":[0.99830496,0.00011604495,0.00036966335,0.000020808948,0.000014460171,0.000003397748,0.0010153177,0.000005217057,0.00015008298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971837,0.00003686308,0.000035396723,0.00008581465,0.000070971735,0.000052557196],"domain_scores_gemma":[0.9981293,0.00017669625,0.0009907343,0.00014882494,0.00017167327,0.0003827733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040577236,0.00032159596,0.00028212118,0.0022875813,0.00039335073,0.0008229536,0.0003240612,0.0002826993,0.00086088263],"category_scores_gemma":[0.00091789966,0.00020608737,0.00029157405,0.0009843863,0.00034409954,0.00026672546,0.0005564857,0.00030502016,0.00021044136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010955155,0.000027111386,0.9787603,0.000017817441,0.00006936802,0.00011040309,0.00008148676,0.00014511686,0.016805844,0.000061383915,0.000104569124,0.0037071188],"study_design_scores_gemma":[0.0000020036243,0.000034592616,0.9987508,0.000004576895,0.000014334418,0.00017543486,0.000025008587,0.00014388704,0.00063600106,0.000032504595,0.0001775108,0.0000033315664],"about_ca_topic_score_codex":0.003434152,"about_ca_topic_score_gemma":0.010024382,"teacher_disagreement_score":0.003434152,"about_ca_system_score_codex":0.00032747284,"about_ca_system_score_gemma":0.00016949784,"threshold_uncertainty_score":0.006828308},"labels":[],"label_agreement":null},{"id":"W2055060539","doi":"10.1086/374590","title":"The Pleiades Reflection Nebula. II. Simple Model Constraints on Dust Properties and Scattering Geometry","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Stars; Pleiades; Astrophysics; Scattering; Nebula; Albedo (alchemy); Light scattering; Astronomy; Optics","score_opus":0.03130293215591216,"score_gpt":0.2546283859864592,"score_spread":0.22332545383054705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055060539","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9199272,0.0011008742,0.04493953,0.00072879903,0.000028380004,0.00012272286,0.0043524164,0.0010084867,0.027791616],"genre_scores_gemma":[0.9841686,0.00042495705,0.0096691,0.0001306263,0.000031526906,0.0000876716,0.0023433839,0.00014181218,0.0030022499],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999871,0.0000337988,0.0000045526886,0.000047161193,0.000020178873,0.000023314311],"domain_scores_gemma":[0.9997551,0.000076892764,0.000051681247,0.0000521164,0.000021553113,0.00004258414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004232573,0.0010478107,0.0007133228,0.00031529917,0.00041037038,0.0010745969,0.0015643948,0.00064613495,0.003539428],"category_scores_gemma":[0.00074333086,0.00062295713,0.0008427158,0.00026336435,0.00046311936,0.0009279348,0.00057962886,0.00058278587,0.0009477766],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023902771,0.00013108073,0.060615152,0.00018050347,0.00014172852,0.00042305866,0.00017568361,0.89168864,0.006071386,0.028777935,0.0030231297,0.008532677],"study_design_scores_gemma":[0.000296873,0.00013074756,0.028533999,0.000031388216,0.00004307943,0.0002844154,0.00006769453,0.93926316,0.0007741652,0.025199136,0.005326893,0.00004843902],"about_ca_topic_score_codex":0.021515388,"about_ca_topic_score_gemma":0.0150938025,"teacher_disagreement_score":0.021515388,"about_ca_system_score_codex":0.0011548355,"about_ca_system_score_gemma":0.0006087991,"threshold_uncertainty_score":0.04278034},"labels":[],"label_agreement":null},{"id":"W2055086077","doi":"10.1086/430595","title":"The X‐Ray Position and Optical Counterpart of the Accretion‐powered Millisecond Pulsar XTE J1814−338","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Black-body radiation; Pulsar; Accretion (finance); X-ray pulsar; Millisecond pulsar; Astronomy; Neutron star; Flux (metallurgy); Observatory; Photon; Radiation; Optics","score_opus":0.006620583051364985,"score_gpt":0.22166366783614452,"score_spread":0.21504308478477954,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055086077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99905604,0.000043136457,0.00005701467,0.00001233264,0.0000024427302,0.0000027862718,0.00019039614,0.0000060458847,0.000629822],"genre_scores_gemma":[0.99832886,0.00006770121,0.00052745995,0.000013736887,0.000015940357,0.0000053774265,0.0005606997,0.0000057197985,0.00047451368],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995816,0.0000020089833,0.0000029704104,0.000013592665,0.000010454449,0.000012723433],"domain_scores_gemma":[0.99971026,0.00001577598,0.00015946994,0.000031362855,0.000025062996,0.000058103848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008578753,0.00024739085,0.00018470123,0.0006352748,0.00041591263,0.00034819852,0.00025290114,0.00020644156,0.001615942],"category_scores_gemma":[0.00026613256,0.00013154156,0.00011566737,0.00043542506,0.00020088634,0.00025340993,0.00034676678,0.00024877148,0.00033050164],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000911352,0.00020950942,0.7343849,0.000089976886,0.000047660436,0.00500619,0.00078642543,0.00033520628,0.21918283,0.0007069447,0.00090706,0.03743194],"study_design_scores_gemma":[0.000020920093,0.00018709073,0.9890709,0.000009289984,0.000015542579,0.0026247147,0.00011157771,0.00022693923,0.0048507936,0.00012744835,0.0027484093,0.000006416624],"about_ca_topic_score_codex":0.0017331039,"about_ca_topic_score_gemma":0.0032515673,"teacher_disagreement_score":0.0017331039,"about_ca_system_score_codex":0.00023197975,"about_ca_system_score_gemma":0.00012130928,"threshold_uncertainty_score":0.0054058433},"labels":[],"label_agreement":null},{"id":"W2055087881","doi":"10.1086/507299","title":"The Stellar Halo and Outer Disk of M33","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Thick disk; Halo; Milky Way; Metallicity; Astronomy; Galactic halo; Stellar population; Galaxy; Population; Velocity dispersion; Dark matter halo; Star formation","score_opus":0.006025246597796477,"score_gpt":0.2016629747786016,"score_spread":0.1956377281808051,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055087881","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990472,0.00011120193,0.00007080285,0.000015602394,6.815163e-7,0.0000023711607,0.00020158684,0.000007798932,0.00054272276],"genre_scores_gemma":[0.9991041,0.0000856114,0.00019412609,0.000017098473,0.0000023889006,0.0000019505487,0.0003938964,0.000004029096,0.00019676516],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994457,0.000005104589,0.0000023438656,0.000011451999,0.00001158834,0.000024884128],"domain_scores_gemma":[0.9998,0.000015858963,0.000057821937,0.000022008982,0.000031192478,0.00007310849],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000091002636,0.00027663144,0.00014080803,0.00074317015,0.0003928727,0.00036900592,0.00012823788,0.00016879673,0.00109497],"category_scores_gemma":[0.00027248566,0.00012311978,0.00016180016,0.0007609976,0.0002290673,0.0001681941,0.0006476247,0.00016144663,0.00039592283],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014138881,0.000019031999,0.96382326,0.00004110688,0.000024415509,0.00039901724,0.0011548413,0.00026067733,0.025092298,0.0002591628,0.0004941539,0.00829069],"study_design_scores_gemma":[0.0000019016719,0.000038026403,0.9969721,0.0000069574867,0.0000074447576,0.00032625385,0.00027253656,0.00019157628,0.00067952665,0.00007549461,0.0014240292,0.0000042081374],"about_ca_topic_score_codex":0.010891366,"about_ca_topic_score_gemma":0.017351974,"teacher_disagreement_score":0.010891366,"about_ca_system_score_codex":0.00037101243,"about_ca_system_score_gemma":0.0001260741,"threshold_uncertainty_score":0.021655977},"labels":[],"label_agreement":null},{"id":"W2055103588","doi":"10.1088/0004-637x/700/1/20","title":"SERENDIPITOUS DISCOVERY OF AN OVERDENSITY OF Lyα EMITTERS AT<i>z</i>∼ 4.8 IN THE CL1604 SUPERCLUSTER FIELD","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Canadian Space Agency; Space Telescope Science Institute; National Astronomical Observatory of Japan; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation","keywords":"Redshift; Physics; Astrophysics; Cosmic variance; Supercluster (genetic); Luminosity; Flux (metallurgy); Field (mathematics); Star formation; Galaxy; Luminosity function; Chemistry","score_opus":0.005603914394005852,"score_gpt":0.21038358259926232,"score_spread":0.20477966820525648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055103588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994942,0.000046673304,0.00006108258,0.000009974919,7.811038e-7,0.0000019324652,0.00006023453,0.0000050002686,0.00032001018],"genre_scores_gemma":[0.9992619,0.000043113305,0.00020538275,0.0000132677105,0.0000061996325,0.000003876665,0.00025500715,0.000002812708,0.0002084862],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997534,0.000022372062,0.000016535503,0.00007516568,0.00006967617,0.00006270715],"domain_scores_gemma":[0.9988978,0.00010037468,0.00052356615,0.00011749478,0.000126399,0.00023436616],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035014906,0.00021189505,0.0002748121,0.0020535619,0.00052274,0.00070444023,0.00047124692,0.00031673693,0.0011515521],"category_scores_gemma":[0.0007874104,0.000188816,0.00017610993,0.0006409914,0.0006855819,0.00038734946,0.0009776535,0.00024386491,0.00025736887],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012907137,0.000026199492,0.9654655,0.000016090966,0.000037397203,0.00029817657,0.0003243811,0.000120337114,0.028066536,0.00012191793,0.000113246104,0.005281283],"study_design_scores_gemma":[0.0000047732988,0.000045895547,0.9977976,0.0000037063974,0.000012504284,0.00037261614,0.00019662837,0.00012343333,0.0009798966,0.00007983202,0.00037934308,0.0000038496755],"about_ca_topic_score_codex":0.0033248446,"about_ca_topic_score_gemma":0.0037890591,"teacher_disagreement_score":0.0033248446,"about_ca_system_score_codex":0.00035772863,"about_ca_system_score_gemma":0.0001585166,"threshold_uncertainty_score":0.0066109896},"labels":[],"label_agreement":null},{"id":"W2055144885","doi":"10.1086/518435","title":"Evidence for Deuterium Astration in the Planetary Nebula Sh 2-216?","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Planetary nebula; Nebula; Spectral line; Line (geometry); Emission nebula; Line-of-sight; Interstellar medium; Ionization; Stars","score_opus":0.038404762870176884,"score_gpt":0.28302727803747574,"score_spread":0.24462251516729885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055144885","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989004,0.000054250097,0.00002207402,0.000016163229,0.0000024832825,0.0000010603555,0.00010998796,0.0000042839893,0.0008892553],"genre_scores_gemma":[0.99937636,0.000045402474,0.000064794905,0.000014977501,0.000006641139,0.000001174734,0.00024497503,0.000002135885,0.0002435427],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999243,0.0000049439136,0.00000647423,0.000025767165,0.000018697145,0.00001986906],"domain_scores_gemma":[0.99981433,0.000010136116,0.0000878877,0.00002047546,0.000016436888,0.000050735518],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009932695,0.00016789447,0.00016042708,0.0004719039,0.00040974942,0.0004322545,0.00022901925,0.000418937,0.0014004955],"category_scores_gemma":[0.00022778123,0.0001608759,0.000112715126,0.00041866396,0.00034640695,0.0002742671,0.0004893111,0.00016709433,0.00037360878],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042280433,0.00007967626,0.85701627,0.00004606856,0.000046474797,0.0012521283,0.00037036565,0.00014481945,0.1348564,0.00033244828,0.00025975806,0.0051726922],"study_design_scores_gemma":[0.000014200573,0.00009550108,0.99187684,0.0000048944344,0.000015238784,0.0009769601,0.00019749503,0.00029264018,0.0048821345,0.00012204132,0.0015171501,0.0000048908973],"about_ca_topic_score_codex":0.0029290107,"about_ca_topic_score_gemma":0.0056462977,"teacher_disagreement_score":0.0029290107,"about_ca_system_score_codex":0.00022150064,"about_ca_system_score_gemma":0.00008649651,"threshold_uncertainty_score":0.0058239102},"labels":[],"label_agreement":null},{"id":"W2055173291","doi":"10.1088/0004-637x/724/2/1182","title":"A BRIGHT, SPATIALLY EXTENDED LENSED GALAXY AT<i>z</i>= 1.7 BEHIND THE CLUSTER RCS2 032727-132623","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Photometry (optics); Galaxy cluster; Type-cD galaxy; Brightest cluster galaxy; Spectral energy distribution; Cluster (spacecraft); Astronomy; Stars","score_opus":0.005865529893422879,"score_gpt":0.20669502049232122,"score_spread":0.20082949059889835,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055173291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.953894,0.00035044758,0.00095103844,0.00071330776,0.00007785722,0.000033140637,0.0023846459,0.00077663927,0.04081892],"genre_scores_gemma":[0.98900175,0.00006174923,0.0009792843,0.00011812181,0.00003184094,0.0000047110457,0.0017302863,0.00003822279,0.008034068],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998667,0.000009232797,0.0000023042337,0.000036270656,0.000034517376,0.000050867537],"domain_scores_gemma":[0.9996544,0.000018085273,0.00004306353,0.000029386163,0.0000374954,0.00021752442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011546163,0.00020258904,0.00025119638,0.0011155083,0.0010631076,0.00072206464,0.00037046944,0.00046855313,0.008780499],"category_scores_gemma":[0.00027155122,0.00016561597,0.00019363883,0.0010136898,0.00042742174,0.00037048123,0.0008974847,0.00039860694,0.0016474662],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015310697,0.00042898324,0.65062714,0.0002417089,0.00028469382,0.007514272,0.006080097,0.0025399104,0.16682191,0.016914599,0.06872817,0.078287445],"study_design_scores_gemma":[0.000039384966,0.00015058285,0.9602131,0.000026171943,0.0000349517,0.001321949,0.0015475828,0.0018812154,0.0032297273,0.0007980322,0.030732788,0.000024402218],"about_ca_topic_score_codex":0.038832866,"about_ca_topic_score_gemma":0.06584753,"teacher_disagreement_score":0.038832866,"about_ca_system_score_codex":0.0006058421,"about_ca_system_score_gemma":0.00047735445,"threshold_uncertainty_score":0.077213705},"labels":[],"label_agreement":null},{"id":"W2055194918","doi":"10.1088/0004-637x/721/1/893","title":"THE FORMATION OF SPHEROIDS IN EARLY-TYPE SPIRALS: CLUES FROM THEIR GLOBULAR CLUSTERS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Astrophysics; Bulge; Physics; Elliptical galaxy; Luminosity; Spiral galaxy; Astronomy; Galaxy; Advanced Camera for Surveys; Hubble space telescope","score_opus":0.00724761808547457,"score_gpt":0.2103625478574473,"score_spread":0.2031149297719727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055194918","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993674,0.000100430676,0.00010038988,0.000010629177,8.642189e-7,0.0000031254044,0.000049755967,0.0000049992527,0.00036254205],"genre_scores_gemma":[0.9995597,0.000059294955,0.00017451956,0.0000043452724,0.0000029072128,0.0000016704879,0.00011189497,0.0000013376131,0.000084317006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998603,0.000019878438,0.0000126701225,0.00003798495,0.00001969397,0.000049480706],"domain_scores_gemma":[0.99900705,0.00015896205,0.00029454604,0.00009686881,0.0001268212,0.0003157487],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043794306,0.00025747513,0.00024731137,0.002137952,0.0005242182,0.000867587,0.0002407333,0.00043859382,0.00061475666],"category_scores_gemma":[0.0012804997,0.00024794554,0.00019359637,0.0009445443,0.00078022026,0.0005607067,0.0008653273,0.00019482058,0.0002955243],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012098732,0.000011520862,0.9902406,0.0000123158625,0.000008800491,0.00013432777,0.0004557417,0.0002095799,0.0063189985,0.00014253397,0.00004383772,0.0023008406],"study_design_scores_gemma":[0.00000350558,0.000037309,0.9982095,0.000003843779,0.000006787,0.00021707913,0.0003485229,0.00029304496,0.0005361489,0.00013681116,0.00020356361,0.000003918212],"about_ca_topic_score_codex":0.006173683,"about_ca_topic_score_gemma":0.009395696,"teacher_disagreement_score":0.006173683,"about_ca_system_score_codex":0.0005586708,"about_ca_system_score_gemma":0.00024424773,"threshold_uncertainty_score":0.012275457},"labels":[],"label_agreement":null},{"id":"W2055208795","doi":"10.1086/592097","title":"Constraining the Physical Parameters of the Circumstellar Disk of χ Ophiuchi","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Balmer series; Astrophysics; Circumstellar disk; Interferometry; Line (geometry); Star (game theory); Constraint (computer-aided design); Astronomy; Emission spectrum; Stars; Spectral line; Geometry","score_opus":0.018778093681977928,"score_gpt":0.2340692193218582,"score_spread":0.2152911256398803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055208795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98142034,0.00016995579,0.011155417,0.00024675584,0.000012980264,0.000023350955,0.00023807617,0.0000705505,0.006662563],"genre_scores_gemma":[0.99693704,0.00009939711,0.00221908,0.000025889034,0.000009022293,0.000024301371,0.00011130313,0.000010567179,0.00056329806],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999436,0.000015098615,0.0000031800355,0.000014328384,0.000008939161,0.000014740419],"domain_scores_gemma":[0.9997354,0.00009587294,0.00006815314,0.000023311259,0.000029921262,0.00004733976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013526283,0.00045826484,0.00044489026,0.00029645694,0.00074125826,0.0011040911,0.00091971044,0.00092196226,0.0012620727],"category_scores_gemma":[0.0013153696,0.0003149711,0.00031881948,0.00035751233,0.0007750482,0.00071210257,0.0006958194,0.0004391303,0.00016598054],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008227552,0.00005342249,0.021121072,0.000032763943,0.000033534878,0.00033804323,0.00016345909,0.96527284,0.0044895727,0.006676337,0.00021050403,0.0015262546],"study_design_scores_gemma":[0.0000432812,0.000037553935,0.003773358,0.0000046742534,0.000017279908,0.000072868694,0.0000743563,0.99303895,0.00030470212,0.0021942675,0.00042661477,0.0000119823835],"about_ca_topic_score_codex":0.03557083,"about_ca_topic_score_gemma":0.011158158,"teacher_disagreement_score":0.03557083,"about_ca_system_score_codex":0.0013409595,"about_ca_system_score_gemma":0.0008424317,"threshold_uncertainty_score":0.07072759},"labels":[],"label_agreement":null},{"id":"W2055321536","doi":"10.1086/378271","title":"The Asymptotic Giant Branch of NGC 205: The Characteristics of Carbon Stars and M Giants Identified from<i>JHK</i>′ Images","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Asymptotic giant branch; Astrophysics; Stars; Carbon star; Astronomy; Red-giant branch; Galaxy; Luminosity; Star formation; Dwarf galaxy; Local Group; Star cluster; Globular cluster","score_opus":0.007059742607889214,"score_gpt":0.20640808898922486,"score_spread":0.19934834638133564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055321536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973968,0.00006786363,0.00018060552,0.00001069295,0.0000010752715,0.0000032716694,0.00030231287,0.000039324317,0.0019979365],"genre_scores_gemma":[0.99900824,0.000018846033,0.00035096187,0.000007831778,0.0000016234794,0.0000016393083,0.00042768993,0.0000037152745,0.00017944371],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999678,0.0000019823653,0.000002007149,0.000007859723,0.000007937051,0.000012311564],"domain_scores_gemma":[0.9998783,0.00001064015,0.000038193848,0.000006301177,0.000016324522,0.000050229915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000058940896,0.00010170061,0.000058886177,0.0010636962,0.00014078089,0.00022399097,0.0000909766,0.00013375872,0.0015084702],"category_scores_gemma":[0.0001225142,0.000053672058,0.0000678331,0.00044577345,0.00013606073,0.00013470321,0.00016394438,0.00009039582,0.00028581888],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002461648,0.000033418517,0.86121076,0.000057589084,0.000025404563,0.00051257387,0.00030706692,0.00023092159,0.11425484,0.00031313463,0.0010563055,0.02175182],"study_design_scores_gemma":[9.48441e-7,0.000012568404,0.9983308,0.0000026693865,0.0000023142054,0.00033235282,0.000056561297,0.00012831147,0.0008564694,0.000014602313,0.00026132987,0.0000011831173],"about_ca_topic_score_codex":0.0046549025,"about_ca_topic_score_gemma":0.014410942,"teacher_disagreement_score":0.0046549025,"about_ca_system_score_codex":0.00015435807,"about_ca_system_score_gemma":0.00008574378,"threshold_uncertainty_score":0.009255648},"labels":[],"label_agreement":null},{"id":"W2055333011","doi":"10.1088/0004-637x/799/2/154","title":"WEATHER ON OTHER WORLDS. II. SURVEY RESULTS: SPOTS ARE UBIQUITOUS ON L AND T DWARFS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":277,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Western University","funders":"","keywords":"Physics; Astrophysics; Brown dwarf; Amplitude; Stellar classification; Surface gravity; Stars; Massive compact halo object; Astronomy; Light curve; Confidence interval; Range (aeronautics); Statistics","score_opus":0.030219155861535365,"score_gpt":0.24957896914453656,"score_spread":0.2193598132830012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055333011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9853498,0.00008595601,0.00029137338,0.000067047455,0.0000042419447,0.000014341489,0.006446194,0.00006395243,0.0076770987],"genre_scores_gemma":[0.9916304,0.00007527266,0.0003721322,0.0000724607,0.00001009439,0.0000150470105,0.0060206186,0.000029799732,0.0017742246],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978775,0.000022418579,0.000013397819,0.00005184525,0.00006535392,0.000059283826],"domain_scores_gemma":[0.998968,0.00012831979,0.0003961895,0.00012965187,0.00017333262,0.0002043807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022498003,0.00013429433,0.00016810287,0.0011677536,0.00036300666,0.0004079039,0.00014330604,0.000115601106,0.002791094],"category_scores_gemma":[0.00086041435,0.00007338356,0.0001699581,0.0012410259,0.00026208386,0.0005024373,0.0006023343,0.00016813604,0.0006876489],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010900791,0.000017394404,0.97759944,0.000036996084,0.00004464849,0.00014143555,0.0005850785,0.0002215172,0.002566888,0.00021224258,0.002589926,0.01587536],"study_design_scores_gemma":[0.000001990019,0.0000109435805,0.9970163,0.00000249511,0.0000072819707,0.0000634441,0.00026127565,0.000100706915,0.00043128373,0.000043954074,0.0020579419,0.0000023588623],"about_ca_topic_score_codex":0.022101615,"about_ca_topic_score_gemma":0.052698568,"teacher_disagreement_score":0.022101615,"about_ca_system_score_codex":0.00029220936,"about_ca_system_score_gemma":0.00018726403,"threshold_uncertainty_score":0.04394591},"labels":[],"label_agreement":null},{"id":"W2055339299","doi":"10.1088/0004-637x/736/2/138","title":"THE 2006–2007 ACTIVE PHASE OF ANOMALOUS X-RAY PULSAR 4U 0142+61: RADIATIVE AND TIMING CHANGES, BURSTS, AND BURST SPECTRAL FEATURES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Pulsar; Astrophysics; Physics; Glitch; Neutron star; Black-body radiation; Phase (matter); Amplitude; Astronomy; Flux (metallurgy); Light curve; Radiation; Detector","score_opus":0.021900103418833604,"score_gpt":0.31189864670758505,"score_spread":0.28999854328875146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055339299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982634,0.0001364183,0.00015373214,0.00003917084,0.000007253856,0.000006837679,0.00013197775,0.000020022619,0.0012412377],"genre_scores_gemma":[0.9987047,0.00010144328,0.0002490002,0.000029411742,0.000025731344,0.000007042875,0.00055408815,0.000008444134,0.0003201119],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998926,0.000011003039,0.000009024039,0.000028653625,0.00003532859,0.000023400864],"domain_scores_gemma":[0.9997552,0.000027448332,0.000105426225,0.000021530928,0.00004134346,0.000049045753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002184992,0.00021466103,0.00021510113,0.00075606676,0.0005197553,0.00076599786,0.00017902644,0.00034066732,0.00061237835],"category_scores_gemma":[0.00051219977,0.00014930117,0.00017919175,0.000633663,0.00044156308,0.00029207315,0.00062826194,0.00034494,0.0001482863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004902167,0.00016988211,0.871778,0.00014347139,0.000114901406,0.0022428792,0.0014269509,0.0018247598,0.07025553,0.0020475278,0.0020303917,0.047475576],"study_design_scores_gemma":[0.000009499667,0.00008741197,0.9945247,0.0000073213228,0.000011187323,0.0008035488,0.00011750749,0.0006461199,0.0014281287,0.00026483703,0.002090695,0.0000090505555],"about_ca_topic_score_codex":0.001681345,"about_ca_topic_score_gemma":0.0026672552,"teacher_disagreement_score":0.001681345,"about_ca_system_score_codex":0.0002757522,"about_ca_system_score_gemma":0.00017812228,"threshold_uncertainty_score":0.0033431053},"labels":[],"label_agreement":null},{"id":"W2055425894","doi":"10.1088/0004-637x/757/2/157","title":"MOLECULAR AND ATOMIC LINE SURVEYS OF GALAXIES. II. UNBIASED ESTIMATES OF THEIR STAR FORMATION MODE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Galaxy; Star formation; Redshift; Interstellar medium; Stellar mass; Line (geometry); Emission spectrum; Galaxy formation and evolution","score_opus":0.013198036963065514,"score_gpt":0.24592924998197901,"score_spread":0.2327312130189135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055425894","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89716196,0.0032174594,0.054378394,0.00048605472,0.000052144762,0.00022121561,0.022078352,0.00071833166,0.021686029],"genre_scores_gemma":[0.9684455,0.0008754349,0.021835566,0.00030983807,0.00007990196,0.00012926914,0.0056685973,0.000026758291,0.0026292368],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99940944,0.00013142312,0.00003200314,0.00017129612,0.00017277944,0.000083023755],"domain_scores_gemma":[0.9987464,0.000118260694,0.0005440879,0.00031832603,0.00017239845,0.00010054512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076918997,0.00024033355,0.00021972785,0.0020951559,0.0002547226,0.0006705764,0.00050742127,0.0004872406,0.0020185038],"category_scores_gemma":[0.001700117,0.00020198552,0.00016501636,0.001563173,0.0002947303,0.000799523,0.00082606985,0.00024163633,0.0014094663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007303157,0.00005351733,0.9128723,0.0001377535,0.000090525864,0.000050301303,0.00036029553,0.0009441296,0.017726157,0.0046924152,0.0017797003,0.061219897],"study_design_scores_gemma":[0.0000061563564,0.00005695733,0.98570514,0.000025640089,0.00002135961,0.00015456643,0.00018712136,0.0021349133,0.0028900795,0.0015586631,0.007245741,0.000013848144],"about_ca_topic_score_codex":0.0033850505,"about_ca_topic_score_gemma":0.007073685,"teacher_disagreement_score":0.0033850505,"about_ca_system_score_codex":0.0003567337,"about_ca_system_score_gemma":0.00021588313,"threshold_uncertainty_score":0.00675261},"labels":[],"label_agreement":null},{"id":"W2055440820","doi":"10.1086/592342","title":"Caught in Formation: The Nuclear‐Cluster‐to‐Be in NGC 2139","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Center (category theory); Star cluster; Protogalaxy; Star formation; Cluster (spacecraft); Galaxy merger","score_opus":0.010934996911621442,"score_gpt":0.20815787272234693,"score_spread":0.19722287581072548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055440820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963952,0.000035260222,0.00009959523,0.00004808143,0.0000072219646,0.0000018534595,0.000097546465,0.000008804142,0.0033065085],"genre_scores_gemma":[0.99926466,0.000011880888,0.00009568297,0.000015379823,0.0000011901931,8.367173e-7,0.00014923255,0.0000029518922,0.00045815352],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992347,0.000004858283,0.000002655385,0.000027471548,0.000013442939,0.000028073819],"domain_scores_gemma":[0.9998815,0.000007762078,0.000029039737,0.0000151868635,0.000022888633,0.00004352871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008640278,0.00007509316,0.00018359313,0.00035350077,0.0014931984,0.00063654326,0.0002513926,0.00021242972,0.0014705207],"category_scores_gemma":[0.0003315431,0.000063643274,0.00007941496,0.0005650844,0.0003685313,0.00018696947,0.0005279885,0.00020824614,0.000391523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041825362,0.00006723454,0.9508468,0.000025605628,0.000028076376,0.0027319873,0.0032272781,0.00031266088,0.02361045,0.0026510989,0.0014979374,0.014582652],"study_design_scores_gemma":[0.0000056961535,0.00003813053,0.9883859,0.000013533635,0.000012294003,0.000954561,0.002122994,0.00025581356,0.0015617706,0.00039231952,0.006250386,0.00000665796],"about_ca_topic_score_codex":0.03634725,"about_ca_topic_score_gemma":0.07473458,"teacher_disagreement_score":0.03634725,"about_ca_system_score_codex":0.0008258853,"about_ca_system_score_gemma":0.00034844675,"threshold_uncertainty_score":0.07227135},"labels":[],"label_agreement":null},{"id":"W2055444796","doi":"10.1086/428494","title":"High‐Resolution Radio Observations of the Colliding‐Wind Binary WR 140","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":144,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Orbital inclination; Circular orbit; Orbital motion; Astronomy; Supergiant; Binary number; Angular momentum; Stars","score_opus":0.017720929385044125,"score_gpt":0.22336379844647963,"score_spread":0.2056428690614355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055444796","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988379,0.00005600183,0.0001153522,0.0000043381283,0.0000013137326,0.0000032190487,0.00013055929,0.000012530412,0.0008389079],"genre_scores_gemma":[0.9969007,0.00006097703,0.00080315204,0.000013099092,0.000008091379,0.000007726004,0.0016536594,0.000008786719,0.0005439057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999424,0.0000037393681,0.0000023462624,0.000013720055,0.000020044057,0.000017679862],"domain_scores_gemma":[0.9998709,0.000013424398,0.00004489761,0.000010926268,0.000017163127,0.00004266859],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013337027,0.00012886671,0.00021290644,0.00035832133,0.0002837708,0.00026361027,0.00019065585,0.0001882955,0.000643291],"category_scores_gemma":[0.0002524622,0.00015657514,0.00010224231,0.00026991343,0.00009197538,0.00013951043,0.00036136052,0.00024031797,0.00020708307],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008892945,0.00038573844,0.6125507,0.000118534896,0.00021080648,0.0011844523,0.0010429743,0.0012694575,0.32438308,0.0005558351,0.0015376788,0.055871483],"study_design_scores_gemma":[0.000018941146,0.00019494166,0.99492633,0.000004344502,0.000016640082,0.0004441032,0.0000838644,0.0004733201,0.0019970224,0.000049381,0.0017847794,0.0000062654635],"about_ca_topic_score_codex":0.0016092905,"about_ca_topic_score_gemma":0.0042019803,"teacher_disagreement_score":0.0016092905,"about_ca_system_score_codex":0.00013880769,"about_ca_system_score_gemma":0.000095674855,"threshold_uncertainty_score":0.0031998158},"labels":[],"label_agreement":null},{"id":"W2055501207","doi":"10.1088/0004-637x/764/2/171","title":"SEARCH FOR A MAGNETIC FIELD VIA CIRCULAR POLARIZATION IN THE WOLF-RAYET STAR EZ CMa","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Stokes parameters; Circular polarization; Astrophysics; Polarization (electrochemistry); Magnetic field; Zeeman effect; Polarization in astronomy; Stars; Scattering; Linear polarization; Optics","score_opus":0.010495151423932671,"score_gpt":0.22630945300535193,"score_spread":0.21581430158141926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055501207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99698704,0.00019410974,0.0012290229,0.00004749602,0.000008770025,0.0000107505475,0.000121744,0.00004309432,0.001357933],"genre_scores_gemma":[0.99745804,0.000054788947,0.0017842107,0.000048864367,0.000016051197,0.0000072732287,0.00024804656,0.0000137866,0.00036893782],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999099,0.000010462162,0.0000044990293,0.000032462813,0.000020621299,0.000022009679],"domain_scores_gemma":[0.9995166,0.000078932186,0.00015810746,0.00005061005,0.000066184,0.00012963107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029495684,0.0002443912,0.00021804613,0.0007122712,0.00041543972,0.0005830998,0.00027534578,0.00044230133,0.0009846409],"category_scores_gemma":[0.0004684613,0.00025588882,0.00015824295,0.0003362351,0.00032469918,0.00027313904,0.0006012291,0.00042202888,0.00043982302],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065853214,0.00014150169,0.50496596,0.00012610544,0.00012733968,0.0013482474,0.00059225236,0.0009159622,0.46460408,0.00094950834,0.0004970553,0.025073413],"study_design_scores_gemma":[0.000071114926,0.00090132526,0.94038475,0.00003128303,0.00007037971,0.0019962867,0.0004522817,0.0054686964,0.044509124,0.00082626916,0.005255168,0.00003336037],"about_ca_topic_score_codex":0.0004162077,"about_ca_topic_score_gemma":0.0008531388,"teacher_disagreement_score":0.0009846409,"about_ca_system_score_codex":0.00015087008,"about_ca_system_score_gemma":0.00013218925,"threshold_uncertainty_score":0.0032939315},"labels":[],"label_agreement":null},{"id":"W2055544206","doi":"10.1086/524769","title":"Simultaneous Multiwavelength Observations of Magnetic Activity in Ultracool Dwarfs. I. The Complex Behavior of the M8.5 Dwarf TVLM 513−46546","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Astrophysics; Physics; Light curve; Balmer series; Astronomy; Rotation period; Flare; Magnetic field; Luminosity; Line (geometry); Emission spectrum; Spectral line; Stars; Galaxy","score_opus":0.030552556776604917,"score_gpt":0.24310790994937204,"score_spread":0.2125553531727671,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055544206","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843985,0.0002742978,0.00017036851,0.000015173154,0.0000055196238,0.0000045642564,0.00033042516,0.000029184024,0.00073055277],"genre_scores_gemma":[0.9979504,0.00010184427,0.00070668623,0.000028606533,0.000016576476,0.0000068236154,0.00070559996,0.0000080834,0.00047555697],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990904,0.000006336196,0.000005970976,0.000029393565,0.000025751393,0.000023532035],"domain_scores_gemma":[0.9997309,0.000019694313,0.00009492714,0.00002104943,0.000028892142,0.00010451092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011381168,0.00020204234,0.00023456842,0.00057737617,0.00024650132,0.00027950364,0.00023132618,0.00020787933,0.0006534415],"category_scores_gemma":[0.00018236278,0.00012622266,0.0001722638,0.0003269394,0.00012267423,0.00015891722,0.0004080577,0.00024212663,0.00024206475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008532445,0.00009954084,0.54849464,0.00010994298,0.00013316494,0.00065604615,0.00058231736,0.00035201118,0.4162271,0.00011357215,0.00044875543,0.031929664],"study_design_scores_gemma":[0.000012876301,0.00017530192,0.99080276,0.000007955004,0.000029104494,0.0005444298,0.0001188258,0.00022684412,0.0068768873,0.000031835163,0.0011664275,0.000006670289],"about_ca_topic_score_codex":0.002056755,"about_ca_topic_score_gemma":0.0057330267,"teacher_disagreement_score":0.002056755,"about_ca_system_score_codex":0.00023855512,"about_ca_system_score_gemma":0.00006580971,"threshold_uncertainty_score":0.004089594},"labels":[],"label_agreement":null},{"id":"W2055623030","doi":"10.1086/308625","title":"Radical Compression of Cosmic Microwave Background Data","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":271,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Multipole expansion; Spectral density; Cosmic background radiation; Robustness (evolution); COSMIC cancer database; Curvature; Anisotropy; Observational cosmology","score_opus":0.021383778803051964,"score_gpt":0.2795512239531651,"score_spread":0.25816744515011314,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055623030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78263724,0.0009977528,0.20096982,0.0014078006,0.00020470556,0.00004594423,0.0016235521,0.0012089689,0.010904239],"genre_scores_gemma":[0.9617482,0.0005638543,0.033938948,0.0002352882,0.00016663045,0.000049170492,0.0018191992,0.00021955527,0.0012593253],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986104,0.00045894907,0.00006855654,0.00023253215,0.0005368793,0.00009264984],"domain_scores_gemma":[0.99235123,0.0034333565,0.00060138677,0.0029080661,0.0006010951,0.000104839346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002881766,0.000421163,0.00042780573,0.0016827015,0.0003859245,0.0016158312,0.0008762889,0.00045348282,0.0011515103],"category_scores_gemma":[0.031042231,0.00026967758,0.00031757477,0.002371279,0.0008613187,0.0017323211,0.0015095875,0.0010950576,0.00060579734],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009282948,0.00011223765,0.13917454,0.00026650072,0.0002375466,0.0006872236,0.0010212003,0.22864628,0.033721853,0.15271962,0.0065786336,0.43590608],"study_design_scores_gemma":[0.000082177576,0.00014984535,0.14111711,0.00013826483,0.00012245428,0.0007603634,0.00034202408,0.68463176,0.042521566,0.10645786,0.023560574,0.000115966795],"about_ca_topic_score_codex":0.0016923477,"about_ca_topic_score_gemma":0.0012597998,"teacher_disagreement_score":0.002881766,"about_ca_system_score_codex":0.00064994814,"about_ca_system_score_gemma":0.00037368055,"threshold_uncertainty_score":0.015240431},"labels":[],"label_agreement":null},{"id":"W2055648194","doi":"10.1088/0004-637x/707/2/1233","title":"PLANETESIMAL AND PROTOPLANET DYNAMICS IN A TURBULENT PROTOPLANETARY DISK: IDEAL UNSTRATIFIED DISKS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Planetesimal; Physics; Protoplanet; Protoplanetary disk; Planetary migration; Planet; Turbulence; Astrophysics; Magnetorotational instability; RADIUS; Accretion (finance); Terrestrial planet; Mechanics; Magnetohydrodynamics; Magnetic field","score_opus":0.007450117000912341,"score_gpt":0.2269774333436926,"score_spread":0.21952731634278028,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055648194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972217,0.000044127075,0.0017280849,0.00003982479,0.0000053079975,0.000009295485,0.00008648169,0.000023823146,0.000841317],"genre_scores_gemma":[0.998209,0.00006192513,0.0013260654,0.000016825907,0.000005005511,0.000018578052,0.00010961422,0.000011811497,0.00024118293],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988437,0.000025524085,0.000010379144,0.000021814862,0.000019998788,0.00003792751],"domain_scores_gemma":[0.9995598,0.00012912572,0.0001035508,0.000052442774,0.00005996348,0.00009508674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002250708,0.00044642726,0.000517824,0.000313571,0.00040628426,0.0009490837,0.0007817686,0.0005469181,0.0006190995],"category_scores_gemma":[0.0015217374,0.0002086142,0.00046749224,0.0004023995,0.0010701637,0.0005951563,0.00066028856,0.00041334645,0.00009121531],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020815374,0.00011988539,0.014167452,0.00004036064,0.000047509944,0.00022383555,0.00014812117,0.97664624,0.0046366826,0.0027701077,0.00010537467,0.00088626076],"study_design_scores_gemma":[0.000063242565,0.00008257366,0.0031819714,0.0000058122237,0.000016699174,0.000026334525,0.00007839082,0.9952225,0.00072249834,0.00051051227,0.000080269325,0.00000924987],"about_ca_topic_score_codex":0.0141508905,"about_ca_topic_score_gemma":0.005847235,"teacher_disagreement_score":0.0141508905,"about_ca_system_score_codex":0.0006715252,"about_ca_system_score_gemma":0.0006603172,"threshold_uncertainty_score":0.028137028},"labels":[],"label_agreement":null},{"id":"W2055654992","doi":"10.1088/0004-637x/780/2/168","title":"LONG-TERM TeV AND X-RAY OBSERVATIONS OF THE GAMMA-RAY BINARY HESS J0632+057","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Office of Science; U.S. Department of Energy; University of Namibia; Centre National de la Recherche Scientifique; Bundesministerium für Bildung und Forschung; Max-Planck-Gesellschaft; Science and Technology Facilities Council; National Research Foundation; Univerzita Karlova v Praze; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Science Foundation Ireland; National Science Foundation","keywords":"Physics; Astrophysics; Light curve; Ephemeris; Orbital period; Astronomy; Cherenkov radiation; Gamma ray; Telescope; Sky; Pulsar; Context (archaeology); Orbit (dynamics); Satellite; Stars; Detector; Optics","score_opus":0.013580741174573994,"score_gpt":0.21758851787870293,"score_spread":0.20400777670412892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055654992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975005,0.00011889839,0.000096407675,0.000030960942,0.00000854156,0.0000057849347,0.0008600421,0.000015616943,0.0013633244],"genre_scores_gemma":[0.9910335,0.00011673039,0.00062629464,0.00005888894,0.000031120995,0.000016465823,0.007271859,0.000017966759,0.00082724215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997888,0.00001841022,0.00001593293,0.00005925631,0.00007143749,0.00004620558],"domain_scores_gemma":[0.9995383,0.000037728383,0.00010397715,0.0000725582,0.00009727127,0.00015015165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037971273,0.00022123913,0.00032369685,0.0007230062,0.000514053,0.00051022583,0.00025499938,0.0003241746,0.00078789756],"category_scores_gemma":[0.00041194036,0.00017289915,0.00020774837,0.0006403219,0.0002722449,0.00038401576,0.00083858444,0.00038274247,0.0005038804],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004425687,0.00026834602,0.9007621,0.00011293506,0.00018486417,0.0010865326,0.0005614934,0.0013203239,0.066614136,0.0004267376,0.0036817528,0.024538254],"study_design_scores_gemma":[0.000007679286,0.00005568801,0.9961966,0.0000067536994,0.000013204375,0.00015234081,0.00007515513,0.00047546747,0.0011457023,0.00004219577,0.0018190439,0.000010075755],"about_ca_topic_score_codex":0.005047131,"about_ca_topic_score_gemma":0.016320212,"teacher_disagreement_score":0.005047131,"about_ca_system_score_codex":0.0003641968,"about_ca_system_score_gemma":0.00026097824,"threshold_uncertainty_score":0.010035515},"labels":[],"label_agreement":null},{"id":"W2055664343","doi":"10.1086/379604","title":"Solar Seismic Models and the Neutrino Predictions","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Helioseismology; Physics; Neutrino; Solar neutrino; Solar neutrino problem; Solar core; Neutrino oscillation; Radiative transfer; Radiation zone; Observatory; Standard solar model; Astrophysics; Magnetic field; Convection zone; Nuclear physics; Optics","score_opus":0.01705809404929689,"score_gpt":0.2589787387001193,"score_spread":0.2419206446508224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055664343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5307512,0.0020283079,0.28075266,0.005607218,0.00036177412,0.000060626226,0.0020936541,0.0012041216,0.17714037],"genre_scores_gemma":[0.9800642,0.00079534354,0.00889072,0.00019361402,0.00013511193,0.000054561988,0.00061913754,0.00019334536,0.009054008],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998939,0.00003485799,0.000004964116,0.000020384712,0.000028108161,0.000017739823],"domain_scores_gemma":[0.99971384,0.000114348375,0.000046628382,0.00003416719,0.00005534364,0.000035716257],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033599418,0.0005257459,0.0003564284,0.00041001337,0.00043292894,0.0012041207,0.00085963507,0.000940653,0.003636329],"category_scores_gemma":[0.0016493716,0.0003504959,0.00045409077,0.00034286155,0.0006453007,0.0011501581,0.0006065363,0.0005839115,0.00064743066],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060653194,0.00003474219,0.0034168025,0.000044632063,0.000029981731,0.00010373476,0.0001592191,0.74536306,0.0014121172,0.23963755,0.0022597346,0.0074778404],"study_design_scores_gemma":[0.000031570467,0.000012976415,0.0017429823,0.000019361814,0.000013176176,0.000032083015,0.000049862327,0.8612884,0.00042781595,0.13300365,0.0033570856,0.000020974221],"about_ca_topic_score_codex":0.00898858,"about_ca_topic_score_gemma":0.003999564,"teacher_disagreement_score":0.00898858,"about_ca_system_score_codex":0.0008997315,"about_ca_system_score_gemma":0.00040775613,"threshold_uncertainty_score":0.017872512},"labels":[],"label_agreement":null},{"id":"W2055728235","doi":"10.1086/429554","title":"The Advanced Camera for Surveys Virgo Cluster Survey. V. Surface Brightness Fluctuation Calibration for Giant and Dwarf Early‐Type Galaxies","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Virgo Cluster; Astrophysics; Globular cluster; Surface brightness fluctuation; Surface brightness; Advanced Camera for Surveys; Dwarf galaxy; Galaxy; Astronomy; Elliptical galaxy; Luminosity; Galaxy cluster; Red-giant branch; Brightest cluster galaxy; Star formation","score_opus":0.010214164091142612,"score_gpt":0.23477236048627487,"score_spread":0.22455819639513225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055728235","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.042451337,0.003155898,0.022904493,0.0012293704,0.00033533445,0.002249079,0.820855,0.016184676,0.090634786],"genre_scores_gemma":[0.113585725,0.0016304828,0.0586411,0.0012848839,0.00026729092,0.0019420641,0.7846639,0.0016927407,0.03629189],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99889755,0.00017684978,0.00006641829,0.00022906064,0.0004901216,0.00013992237],"domain_scores_gemma":[0.9979303,0.00008772385,0.00043137578,0.00046568617,0.00082792126,0.0002569932],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00193695,0.00083002454,0.00064651563,0.00577265,0.00054275524,0.0009187786,0.001009073,0.0005256898,0.012867362],"category_scores_gemma":[0.0024496885,0.00040783797,0.0004207745,0.004660121,0.00022294396,0.0009855669,0.0011681526,0.0008929537,0.015309848],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029263564,0.00015416418,0.07902534,0.0003161817,0.00014289627,0.000053577518,0.00015249327,0.0006158266,0.005127425,0.0045151855,0.7832581,0.12634614],"study_design_scores_gemma":[0.00020260194,0.000074965654,0.426533,0.00012877819,0.00007769196,0.00015295426,0.0001344548,0.0030713517,0.0029038414,0.0025233258,0.5641221,0.000074980526],"about_ca_topic_score_codex":0.048289686,"about_ca_topic_score_gemma":0.04471192,"teacher_disagreement_score":0.048289686,"about_ca_system_score_codex":0.0013494695,"about_ca_system_score_gemma":0.0012362389,"threshold_uncertainty_score":0.09601724},"labels":[],"label_agreement":null},{"id":"W2055976583","doi":"10.1086/504413","title":"Toward a Cosmological Hubble Diagram for Type II‐P Supernovae","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"Physics; Redshift; Astrophysics; Supernova; Photometry (optics); Galaxy; Observatory; Hubble's law; Dark energy; Brightness; Astronomy; Cosmology; Stars","score_opus":0.028560685536657783,"score_gpt":0.26001867252342087,"score_spread":0.2314579869867631,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2055976583","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3137424,0.0018712908,0.6310027,0.00080679794,0.00018279137,0.00022742484,0.0029580703,0.0027071615,0.046501353],"genre_scores_gemma":[0.77279246,0.00042884029,0.2227143,0.00006599662,0.00011713524,0.00013991886,0.0020189073,0.00021826824,0.0015040851],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995741,0.00015829218,0.00002774634,0.000108413566,0.00009334957,0.000038140744],"domain_scores_gemma":[0.9971131,0.0008280516,0.0008444212,0.00032260583,0.00049013057,0.00040177023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010613373,0.00047654833,0.00031822003,0.00390398,0.0006299771,0.0014822821,0.0007729513,0.00039910842,0.002810383],"category_scores_gemma":[0.0071746265,0.00024185714,0.00027551857,0.0013496957,0.0006280416,0.0019420063,0.0009799467,0.0009832002,0.00081616506],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021002434,0.000116455136,0.1711031,0.00020094374,0.00008201499,0.00028960744,0.0010486536,0.024747672,0.0075321575,0.56071275,0.014326385,0.21963027],"study_design_scores_gemma":[0.000084498315,0.00017115635,0.21229444,0.0001406777,0.000044686032,0.0009630337,0.00037203165,0.14619116,0.0036882034,0.516936,0.11895946,0.00015464959],"about_ca_topic_score_codex":0.0029016605,"about_ca_topic_score_gemma":0.0020852447,"teacher_disagreement_score":0.00390398,"about_ca_system_score_codex":0.00093060324,"about_ca_system_score_gemma":0.00062439445,"threshold_uncertainty_score":0.009401679},"labels":[],"label_agreement":null},{"id":"W2056067080","doi":"10.1088/0004-637x/766/1/27","title":"THE EFFECT OF MAGNETIC FIELDS AND AMBIPOLAR DIFFUSION ON CORE MASS FUNCTIONS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Diffusion; Core (optical fiber); Magnetic field; Physics; Nuclear physics; Plasma; Optics; Thermodynamics; Quantum mechanics","score_opus":0.0050028451376710765,"score_gpt":0.20829746191775278,"score_spread":0.2032946167800817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056067080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947614,0.00010097694,0.0038762335,0.00007398997,0.0000041318103,0.000005655255,0.00009450564,0.00007087757,0.0010122913],"genre_scores_gemma":[0.99963975,0.000024683068,0.00022544224,0.000006743723,0.0000022167421,0.0000021119645,0.000042183055,0.000009471705,0.000047292724],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99975044,0.00009607199,0.00001481146,0.00005880351,0.0000325178,0.000047314064],"domain_scores_gemma":[0.9935882,0.0047096987,0.00079808076,0.00039348524,0.00025572252,0.00025473844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008887948,0.0003349833,0.00019490658,0.00051330705,0.0002208027,0.00051768456,0.0003290667,0.00032371873,0.00063563423],"category_scores_gemma":[0.0090521155,0.00023263092,0.00023810158,0.00027444604,0.00062842097,0.00046664296,0.0004845608,0.00028498707,0.000095659976],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010361627,0.000114924704,0.19081666,0.000111010566,0.00016848689,0.000699664,0.00021144301,0.69327754,0.09199599,0.007039089,0.00035845523,0.01417067],"study_design_scores_gemma":[0.000059887363,0.00020423166,0.1262256,0.000020333331,0.000063139996,0.00022938155,0.00006381278,0.8378248,0.032105993,0.0027818652,0.00036833077,0.000052532625],"about_ca_topic_score_codex":0.0013406888,"about_ca_topic_score_gemma":0.000901604,"teacher_disagreement_score":0.0013406888,"about_ca_system_score_codex":0.00043453957,"about_ca_system_score_gemma":0.0001631601,"threshold_uncertainty_score":0.0047004223},"labels":[],"label_agreement":null},{"id":"W2056227024","doi":"10.1086/512361","title":"Protostellar Outflow‐driven Turbulence","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Outflow; Turbulence; Physics; Astrophysics; Cascade; Energy cascade; Scaling; Cluster (spacecraft); Turbulence kinetic energy; Star formation; Supersonic speed; K-epsilon turbulence model; Mechanics; Stars; Meteorology; Geometry; Chemistry","score_opus":0.00980155483835358,"score_gpt":0.24600932833724906,"score_spread":0.2362077734988955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056227024","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9341592,0.00020667393,0.040991474,0.00041901172,0.00008078145,0.000058144145,0.00022679908,0.00039501762,0.023462841],"genre_scores_gemma":[0.9970994,0.00007497714,0.0009501081,0.000045688197,0.000015960055,0.000019937192,0.00005110452,0.000013499316,0.0017295075],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999479,0.000006850138,0.0000023106973,0.0000126160685,0.00000836791,0.000021988195],"domain_scores_gemma":[0.99991465,0.0000064737965,0.00002855161,0.000012272261,0.000008364207,0.000029601872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059538637,0.000342432,0.00024136026,0.0001212044,0.0003503823,0.0006526722,0.0004079307,0.0004749149,0.0010671411],"category_scores_gemma":[0.00018440088,0.00015245735,0.00047398914,0.00011672429,0.0005143652,0.0003226164,0.0005704524,0.0003488591,0.00020874193],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021635425,0.00018484824,0.037195303,0.0000484709,0.00006302402,0.0007953087,0.0002443308,0.77234197,0.059016153,0.12054936,0.0018578961,0.00748689],"study_design_scores_gemma":[0.00012476476,0.00011381257,0.019448675,0.000007712001,0.000029215162,0.0001879504,0.00005890492,0.95991665,0.0032495814,0.014303709,0.0025285245,0.0000303371],"about_ca_topic_score_codex":0.0056951423,"about_ca_topic_score_gemma":0.0023357593,"teacher_disagreement_score":0.0056951423,"about_ca_system_score_codex":0.0006737104,"about_ca_system_score_gemma":0.000541945,"threshold_uncertainty_score":0.011323988},"labels":[],"label_agreement":null},{"id":"W2056285996","doi":"10.1088/0004-637x/727/2/107","title":"SUBLUMINOUS TYPE Ia SUPERNOVAE AT HIGH REDSHIFT FROM THE SUPERNOVA LEGACY SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Defence Research and Development Canada; Herzberg Institute of Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Supernova; Redshift; Galaxy; Astronomy; Population","score_opus":0.030043030367984915,"score_gpt":0.23758414970598637,"score_spread":0.20754111933800146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056285996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957302,0.00023305687,0.0002818547,0.000008501053,0.0000023586906,0.0000061672904,0.0027358641,0.000024519122,0.0009774179],"genre_scores_gemma":[0.9848002,0.00043096583,0.0005754618,0.000011947344,0.000013993259,0.000007815543,0.0131563,0.00001606782,0.0009873429],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984694,0.000018772344,0.000016120788,0.00004394208,0.000040549963,0.00003373329],"domain_scores_gemma":[0.9985349,0.00014386073,0.000718249,0.00020741862,0.00014446277,0.0002510299],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042096752,0.00023638971,0.00024006286,0.0020577994,0.00017182548,0.000569264,0.00022370818,0.00012058074,0.0015535294],"category_scores_gemma":[0.0013164274,0.00013947027,0.00029608046,0.0010248707,0.00012661226,0.00029772305,0.0007894457,0.00022385283,0.000620687],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005402509,0.000010594433,0.99144167,0.000010993556,0.000054926597,0.00006006536,0.00008180099,0.00011806074,0.0013053778,0.00007213,0.0001916708,0.006598563],"study_design_scores_gemma":[0.0000011388381,0.000014500246,0.998825,0.0000017102053,0.000012924279,0.0001800115,0.000018707107,0.00007119541,0.00018720215,0.000026048025,0.0006599717,0.0000015801766],"about_ca_topic_score_codex":0.004671537,"about_ca_topic_score_gemma":0.008406571,"teacher_disagreement_score":0.004671537,"about_ca_system_score_codex":0.00020028903,"about_ca_system_score_gemma":0.00012904489,"threshold_uncertainty_score":0.009288728},"labels":[],"label_agreement":null},{"id":"W2056287285","doi":"10.1086/511765","title":"The Origin and Evolution of the Mass-Metallicity Relationship for Galaxies: Results from Cosmological <i>N</i> -Body Simulations","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":262,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Supernova; Metallicity; Galaxy; Stars; Star formation; Galaxy formation and evolution; Redshift; Baryon; Astronomy","score_opus":0.016218112688671432,"score_gpt":0.24614061390441608,"score_spread":0.22992250121574465,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056287285","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942023,0.00010016157,0.0014036224,0.00024642854,0.000013346714,0.00001989326,0.00092021434,0.00021491278,0.0028790303],"genre_scores_gemma":[0.9959615,0.000062378356,0.002344961,0.000075627024,0.000010925832,0.000025994834,0.0010232405,0.000096970616,0.00039850952],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99976987,0.0000692165,0.00001451078,0.0000420466,0.000043380925,0.000061006733],"domain_scores_gemma":[0.9974253,0.0014324368,0.00035095788,0.00022772227,0.00021976788,0.00034380853],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008305558,0.00072059565,0.00061158364,0.0007234228,0.0006354992,0.00094361877,0.0012849695,0.001359474,0.0016469345],"category_scores_gemma":[0.0056232754,0.0004954091,0.00081380503,0.00076371245,0.00090396905,0.0005921518,0.0007287039,0.0010529526,0.00022243566],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025759268,0.00020795756,0.05823981,0.0000692464,0.00018867535,0.0002458257,0.00016936168,0.9290679,0.004375179,0.0032422594,0.0013329581,0.0026032096],"study_design_scores_gemma":[0.00009294369,0.00006118757,0.01016553,0.000012254715,0.00003089279,0.000031815067,0.00006528849,0.9870754,0.0010604091,0.0010144796,0.00037066455,0.000019174015],"about_ca_topic_score_codex":0.022643067,"about_ca_topic_score_gemma":0.018776532,"teacher_disagreement_score":0.022643067,"about_ca_system_score_codex":0.0012273559,"about_ca_system_score_gemma":0.0006642368,"threshold_uncertainty_score":0.045022547},"labels":[],"label_agreement":null},{"id":"W2056314771","doi":"10.1088/0004-637x/695/2/1082","title":"STOCHASTIC SELF-ENRICHMENT, PRE-ENRICHMENT, AND THE FORMATION OF GLOBULAR CLUSTERS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Metallicity; Astrophysics; Globular cluster; Supernova; Physics; Cluster (spacecraft); Galaxy; Computer science","score_opus":0.005856971992605174,"score_gpt":0.2312526959360309,"score_spread":0.22539572394342572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056314771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.61400825,0.0007364539,0.359542,0.0024898688,0.00009545362,0.00010536792,0.0004505632,0.00040877485,0.022163333],"genre_scores_gemma":[0.97321004,0.00038436355,0.012222921,0.00021716022,0.000054766555,0.00012137358,0.0001595952,0.000081886705,0.013547932],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998516,0.00003307067,0.000004824857,0.000034426346,0.000027321123,0.000048780614],"domain_scores_gemma":[0.999313,0.0002194976,0.00016979376,0.00006586743,0.000095766285,0.00013609848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045936066,0.00045223694,0.0005375448,0.0004894452,0.0007728946,0.0010682559,0.0022184744,0.0013174433,0.0026784167],"category_scores_gemma":[0.001948251,0.00039692956,0.0008230759,0.00039040507,0.0014593042,0.0015684643,0.0012641564,0.0008918271,0.0004808393],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031681742,0.00002567352,0.0043524634,0.000025294587,0.000022100827,0.00018340838,0.00015991977,0.8442385,0.0018076806,0.14620419,0.0010360272,0.0019130878],"study_design_scores_gemma":[0.000018429228,0.000018160059,0.0009905259,0.000006516358,0.000008214173,0.00004968618,0.000023557994,0.9547844,0.00016916072,0.043075893,0.00084142736,0.000013936168],"about_ca_topic_score_codex":0.019145131,"about_ca_topic_score_gemma":0.008551407,"teacher_disagreement_score":0.019145131,"about_ca_system_score_codex":0.001953285,"about_ca_system_score_gemma":0.0010620402,"threshold_uncertainty_score":0.0380674},"labels":[],"label_agreement":null},{"id":"W2056336778","doi":"10.1088/0004-637x/762/1/58","title":"A LONG-PERIOD TOTALLY ECLIPSING BINARY STAR AT THE TURNOFF OF THE OPEN CLUSTER NGC 6819 DISCOVERED WITH<i>KEPLER</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Open cluster; Photometry (optics); Star cluster; Primary (astronomy); Binary star; Eclipse; Stars; Cluster (spacecraft); RADIUS","score_opus":0.01174533650303215,"score_gpt":0.23037584116808207,"score_spread":0.21863050466504994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056336778","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989423,0.00007872721,0.00013508456,0.000022834838,0.000005918691,0.0000025938546,0.00008553609,0.000010566574,0.0007164326],"genre_scores_gemma":[0.99919134,0.000053346732,0.0002409862,0.00002083374,0.000012483642,0.0000020913417,0.00023483647,0.0000028979882,0.00024113726],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999275,0.0000033094966,0.000002676733,0.000021799915,0.000018518187,0.000026262283],"domain_scores_gemma":[0.99973863,0.000018161432,0.00010744362,0.000015552529,0.00002317161,0.00009699468],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000055331308,0.00023523583,0.0001936296,0.00075306103,0.0006696449,0.0004022733,0.0003397974,0.0002900361,0.0006043818],"category_scores_gemma":[0.00026738134,0.000104806095,0.00009358924,0.0004245963,0.0005014999,0.00022873205,0.0005027604,0.00024657257,0.0002328224],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024102727,0.00007200457,0.9215009,0.00004420279,0.000039516784,0.0104247285,0.00071913266,0.00014747563,0.048432082,0.00060598843,0.001005885,0.016767075],"study_design_scores_gemma":[0.0000065082186,0.00015875463,0.9802012,0.0000097321545,0.000030150344,0.012153941,0.00032404016,0.00031122542,0.0033114976,0.00019568614,0.0032858697,0.000011375004],"about_ca_topic_score_codex":0.004893735,"about_ca_topic_score_gemma":0.010288515,"teacher_disagreement_score":0.004893735,"about_ca_system_score_codex":0.00039411924,"about_ca_system_score_gemma":0.00011844446,"threshold_uncertainty_score":0.009730458},"labels":[],"label_agreement":null},{"id":"W2056436934","doi":"10.1088/0004-637x/761/2/122","title":"EXTRACTING PLANET MASS AND ECCENTRICITY FROM TTV DATA","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":335,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planet; Physics; Eccentricity (behavior); Amplitude; Astrophysics; Mean motion; Outer planets; Planetary mass; Kepler's laws of planetary motion; Kepler; Planetary system; Quantum mechanics","score_opus":0.02867459284215393,"score_gpt":0.24906958672740354,"score_spread":0.2203949938852496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056436934","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99108046,0.00009381114,0.0057758917,0.000014368852,0.000009426604,0.00001692595,0.0012554532,0.00018376457,0.0015698937],"genre_scores_gemma":[0.99437994,0.00003064253,0.0036407572,0.0000033243998,0.0000064529863,0.000012325064,0.0016592764,0.000022014989,0.00024534317],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999696,0.00004067455,0.000037277823,0.00008416773,0.000087702574,0.000054158998],"domain_scores_gemma":[0.9984939,0.0005053523,0.00038826728,0.00025356252,0.00024861787,0.00011022939],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031913727,0.00036227962,0.00032188764,0.0033154278,0.00031713035,0.00049142714,0.0003055927,0.0003583203,0.0010980791],"category_scores_gemma":[0.004120222,0.00020691214,0.0002867931,0.0019774907,0.00016498455,0.00053249113,0.00062597607,0.0002322772,0.0008291517],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004884634,0.000048825917,0.8326182,0.00013399466,0.00013367391,0.00057467824,0.00067853986,0.0064712805,0.08222027,0.00075424416,0.00081148767,0.075066395],"study_design_scores_gemma":[0.000014081199,0.00014737275,0.9425356,0.000020421505,0.000046411733,0.0009611523,0.00024876447,0.028837608,0.02382836,0.0006997889,0.0026199613,0.000040511855],"about_ca_topic_score_codex":0.0011512964,"about_ca_topic_score_gemma":0.001512913,"teacher_disagreement_score":0.0033154278,"about_ca_system_score_codex":0.00024315887,"about_ca_system_score_gemma":0.00015134267,"threshold_uncertainty_score":0.0036733747},"labels":[],"label_agreement":null},{"id":"W2056653166","doi":"10.1088/0004-637x/749/1/7","title":"THIRD COMPONENT SEARCH AND ABUNDANCES OF THE VERY DUSTY SHORT-PERIOD BINARY BD +20°307","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Stars; Radial velocity; Binary number; Orbital period; Binary star; Orbital elements; Lithium (medication); Astronomy","score_opus":0.01874300389826114,"score_gpt":0.24495905428596534,"score_spread":0.2262160503877042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056653166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917775,0.0000917356,0.0001483444,0.000007862461,0.0000022888703,0.000002027815,0.000071782575,0.0000073729516,0.0004908394],"genre_scores_gemma":[0.99882334,0.000034335822,0.0005310771,0.0000060573334,0.0000029473208,0.0000026184632,0.00036828517,0.0000058911937,0.00022535525],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998878,0.000008337099,0.0000074636187,0.000027126276,0.000038431856,0.0000308602],"domain_scores_gemma":[0.9997075,0.000034376477,0.000096695476,0.000023276376,0.000051299703,0.00008695321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001672539,0.00015008579,0.0002792216,0.0012876826,0.0006711189,0.0006036688,0.00021266073,0.00025539185,0.0009197372],"category_scores_gemma":[0.00040157596,0.000170914,0.00013013801,0.00087015016,0.00020549243,0.00021448775,0.00037945545,0.00023070857,0.00023621057],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007347033,0.00012304171,0.7692203,0.000064694264,0.000040147024,0.00045344082,0.00047807102,0.00053309026,0.20746334,0.00059504365,0.00029342234,0.020000694],"study_design_scores_gemma":[0.000014464755,0.00010492754,0.98391217,0.000007521261,0.000021300313,0.00037819133,0.00022145452,0.0014262423,0.01277361,0.00013713415,0.0009946147,0.000008277231],"about_ca_topic_score_codex":0.0035963252,"about_ca_topic_score_gemma":0.0071469466,"teacher_disagreement_score":0.0035963252,"about_ca_system_score_codex":0.00043966185,"about_ca_system_score_gemma":0.00025903128,"threshold_uncertainty_score":0.007150829},"labels":[],"label_agreement":null},{"id":"W2056742289","doi":"10.1088/0004-637x/779/1/80","title":"THE GEMINI NICI PLANET-FINDING CAMPAIGN: THE COMPANION DETECTION PIPELINE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Exoplanet; Planet; Stars; Physics; Astronomy; Pipeline (software); Computer science; Telescope; Contrast (vision); Artificial intelligence; Computer vision; Operating system","score_opus":0.012114103125097137,"score_gpt":0.2223687377779818,"score_spread":0.21025463465288466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056742289","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.30803737,0.0011902889,0.33790386,0.0010108986,0.00033500316,0.002774939,0.17343451,0.13029936,0.04501377],"genre_scores_gemma":[0.2107825,0.00024503635,0.45726687,0.00030812467,0.00017209702,0.0011775634,0.31210142,0.006038467,0.011908007],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99941134,0.000044538057,0.00002814418,0.00018157158,0.00022717517,0.000107210115],"domain_scores_gemma":[0.9991762,0.00007457393,0.00006879815,0.00030049912,0.0002907018,0.000089060464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009835964,0.0008763282,0.0006265631,0.0019443785,0.00072817254,0.001231864,0.0010335216,0.00063496584,0.008915625],"category_scores_gemma":[0.0018092686,0.0005368947,0.0007486873,0.0014413334,0.00018278598,0.0008598751,0.0012351513,0.0007273992,0.009079287],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015500623,0.00046361942,0.07213471,0.0006057518,0.00039180872,0.00039095737,0.000743348,0.013380802,0.12965506,0.002042084,0.2110465,0.56759524],"study_design_scores_gemma":[0.0004533656,0.0004937243,0.34373277,0.00009044472,0.00026975875,0.00087385124,0.0004064693,0.17762809,0.11154714,0.0034077005,0.3608746,0.00022219078],"about_ca_topic_score_codex":0.01366033,"about_ca_topic_score_gemma":0.021861436,"teacher_disagreement_score":0.01366033,"about_ca_system_score_codex":0.00076273707,"about_ca_system_score_gemma":0.00113732,"threshold_uncertainty_score":0.029825747},"labels":[],"label_agreement":null},{"id":"W2056888177","doi":"10.1086/591653","title":"DA 495: An Aging Pulsar Wind Nebula","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Manitoba; University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Pulsar; Nebula; Pulsar wind nebula; Supernova remnant; Astronomy; Spectral index; Galactic plane; Supernova; Stars; Spectral line","score_opus":0.014642148622465595,"score_gpt":0.23518141150823496,"score_spread":0.22053926288576936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056888177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996031,0.00035332874,0.00013785697,0.000032950145,0.000014753907,0.000005622866,0.00028894778,0.000015900163,0.0031195993],"genre_scores_gemma":[0.998178,0.00011332539,0.0001155764,0.000044185737,0.000010006592,0.0000014385813,0.00039935054,0.0000044995663,0.0011335965],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999455,0.0000014540614,0.000002425439,0.000016258453,0.000015574422,0.00001870546],"domain_scores_gemma":[0.9999372,0.000001844127,0.000011991253,0.000004872762,0.000009475915,0.000034658846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000041300686,0.00016455534,0.00013518559,0.0005578538,0.0005741724,0.00048600725,0.0002813114,0.00018145288,0.0018104834],"category_scores_gemma":[0.00007839519,0.00005462026,0.00009433363,0.0003516377,0.00021739306,0.00020501354,0.00027151965,0.00014641356,0.00044985025],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062425574,0.00020898237,0.74262416,0.000058567275,0.00009021453,0.007938058,0.00051121885,0.0003629933,0.20962487,0.0011032469,0.0017689524,0.03508445],"study_design_scores_gemma":[0.0000065422455,0.00010750535,0.9864166,0.0000051791344,0.000017715856,0.0030129768,0.00017289228,0.00019062658,0.0028176508,0.000070705726,0.0071756444,0.0000059834283],"about_ca_topic_score_codex":0.023112848,"about_ca_topic_score_gemma":0.037495255,"teacher_disagreement_score":0.023112848,"about_ca_system_score_codex":0.00057035265,"about_ca_system_score_gemma":0.00013271453,"threshold_uncertainty_score":0.04595661},"labels":[],"label_agreement":null},{"id":"W2056918667","doi":"10.1088/0004-637x/728/2/86","title":"CONFIRMATION OF IGR J01363+6610 AS A Be X-RAY BINARY WITH VERY LOW QUIESCENT X-RAY LUMINOSITY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Luminosity; Binary number; Flux (metallurgy); Photon; Stellar classification; Eddington luminosity; X-ray binary; Limit (mathematics); Luminosity function","score_opus":0.017890482978286045,"score_gpt":0.21729607946116225,"score_spread":0.1994055964828762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056918667","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960381,0.00035143923,0.00036076803,0.00016311242,0.000040195777,0.00001749915,0.00014335806,0.00003056268,0.00285489],"genre_scores_gemma":[0.99814,0.00011613249,0.00047557952,0.00013599553,0.000027677903,0.000005749197,0.00042674848,0.000007288266,0.0006647475],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997099,0.000026982727,0.00003205259,0.000063225154,0.00008329436,0.00008448206],"domain_scores_gemma":[0.99886024,0.00012773494,0.00034883426,0.0000684677,0.00013942191,0.00045530728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006102133,0.00049500156,0.00064022484,0.00096706057,0.0008017378,0.0009205355,0.00079419103,0.0009365794,0.0030116546],"category_scores_gemma":[0.0010043895,0.00025198268,0.00036754226,0.0008298181,0.00067080645,0.00031197033,0.0006934052,0.00060586835,0.0014508663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044766345,0.00023829388,0.86822116,0.00019542557,0.000050045524,0.01512797,0.00084604387,0.00011673301,0.10500399,0.00084228464,0.0008526038,0.008057789],"study_design_scores_gemma":[0.00002466586,0.0003279692,0.9772495,0.000042196763,0.0000314974,0.014742332,0.0006456843,0.0003992875,0.0040983893,0.00030328025,0.002123172,0.000012114804],"about_ca_topic_score_codex":0.0024254795,"about_ca_topic_score_gemma":0.004493834,"teacher_disagreement_score":0.0030116546,"about_ca_system_score_codex":0.00041928623,"about_ca_system_score_gemma":0.00028270332,"threshold_uncertainty_score":0.010074973},"labels":[],"label_agreement":null},{"id":"W2056935071","doi":"10.1088/0004-637x/693/2/1696","title":"ONE-DIMENSIONAL DYNAMICAL MODELS OF THE CARINA NEBULA BUBBLE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Bubble; Nebula; Luminosity; RADIUS; Radiation pressure; Surface brightness; Stellar mass; Mechanics; Star formation; Stars; Galaxy","score_opus":0.011827932422515125,"score_gpt":0.2275946432309039,"score_spread":0.21576671080838877,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056935071","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9098292,0.0008767306,0.033635154,0.0010045407,0.00012988526,0.00016368787,0.0010283745,0.00039476607,0.05293765],"genre_scores_gemma":[0.98816353,0.0002837954,0.003472523,0.00009008843,0.00005697384,0.00013828446,0.00027795354,0.00007621776,0.0074406015],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989307,0.00002236047,0.0000059010363,0.000024736955,0.000021219503,0.000032601754],"domain_scores_gemma":[0.9995542,0.00011917523,0.000092917566,0.000032329986,0.000061436665,0.00013977967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024395331,0.0005613078,0.0006846984,0.00056558615,0.0009394837,0.001581463,0.0021452561,0.0011740867,0.006530182],"category_scores_gemma":[0.0009031701,0.0004666957,0.00074362673,0.00026714258,0.0009540479,0.0011977969,0.0011472792,0.00081659533,0.00056044705],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017552807,0.00013996413,0.009400548,0.000109740984,0.000071780436,0.00071958057,0.0007797082,0.81467086,0.0055847988,0.16291822,0.0018237998,0.003605408],"study_design_scores_gemma":[0.0000766935,0.000039391973,0.0015986875,0.000008816721,0.000013640766,0.00007712493,0.0001054601,0.98289996,0.0001897377,0.013785143,0.0011795169,0.000025830608],"about_ca_topic_score_codex":0.019971292,"about_ca_topic_score_gemma":0.00670387,"teacher_disagreement_score":0.019971292,"about_ca_system_score_codex":0.0017885818,"about_ca_system_score_gemma":0.0007160218,"threshold_uncertainty_score":0.039710045},"labels":[],"label_agreement":null},{"id":"W2056992591","doi":"10.1086/426133","title":"Globular Clusters with Dark Matter Halos. II. Evolution in a Tidal Field","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Dark matter; Dark matter halo; Astronomy; Galaxy cluster; Cuspy halo problem; Hot dark matter; Halo; Galaxy; Cosmology; Dark energy","score_opus":0.003458011992374724,"score_gpt":0.19071349320627207,"score_spread":0.18725548121389735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2056992591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980451,0.00007214319,0.00074240053,0.000045434237,0.0000054059014,0.000013551711,0.0001147153,0.000045574187,0.0009158125],"genre_scores_gemma":[0.9981165,0.000050247727,0.0010587968,0.000022043743,0.0000029456733,0.0000056907056,0.00021412375,0.000013203354,0.00051654567],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998313,0.00004537963,0.000008774083,0.000028806451,0.00003578858,0.00004989432],"domain_scores_gemma":[0.99898106,0.00022062472,0.00019982371,0.00022058096,0.00013593565,0.0002420137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005311458,0.00038669052,0.0002870675,0.0004151424,0.00073186454,0.0008772455,0.0006329821,0.000545333,0.0007789681],"category_scores_gemma":[0.0019202251,0.00030006972,0.0003614527,0.00057786173,0.00080152124,0.00075294194,0.0008198247,0.0003972576,0.00013815446],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007438318,0.00020963477,0.28770265,0.00008948059,0.00019768046,0.00063664245,0.00042357267,0.67449147,0.016344415,0.011553062,0.0010522538,0.0065552965],"study_design_scores_gemma":[0.00026113776,0.00035331736,0.10848836,0.000017769647,0.00007514444,0.0003087419,0.00043704704,0.867517,0.008200484,0.012156856,0.0021254297,0.000058708978],"about_ca_topic_score_codex":0.017133294,"about_ca_topic_score_gemma":0.011468624,"teacher_disagreement_score":0.017133294,"about_ca_system_score_codex":0.0012644148,"about_ca_system_score_gemma":0.0005314096,"threshold_uncertainty_score":0.034067154},"labels":[],"label_agreement":null},{"id":"W2057004724","doi":"10.1088/0004-637x/729/1/40","title":"FLUORINE AND SODIUM IN C-RICH LOW-METALLICITY STARS,","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; TRIUMF","funders":"","keywords":"Stars; Metallicity; Astrophysics; Physics; Abundance (ecology); Spectral line; Low Mass; Asymptotic giant branch; Astronomy; Biology","score_opus":0.014698364229285436,"score_gpt":0.2119496251321378,"score_spread":0.19725126090285236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057004724","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99928707,0.00018125318,0.00008638158,0.0000063180123,6.734304e-7,8.018759e-7,0.00010699977,0.000003848086,0.0003266196],"genre_scores_gemma":[0.9992612,0.00006316593,0.00024656867,0.000008445425,0.0000017153469,9.881072e-7,0.00027237777,0.0000026857053,0.00014289898],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998832,0.000010056567,0.000011290524,0.000050423154,0.000026268583,0.000018741272],"domain_scores_gemma":[0.99969816,0.00004756,0.0001416671,0.000023020983,0.0000446144,0.000045012755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017830532,0.00021725609,0.00020087273,0.0010355514,0.00045877422,0.00041669802,0.00021389141,0.0004357184,0.00069128355],"category_scores_gemma":[0.00041275364,0.00010964379,0.00017163226,0.00049619976,0.00032959544,0.0002684319,0.0003421695,0.000093971,0.00026219484],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053983775,0.000027060882,0.8850494,0.000066435976,0.0000657277,0.00020742451,0.00018214164,0.0003238666,0.106786706,0.000114211456,0.000051204355,0.0065860595],"study_design_scores_gemma":[0.000011779648,0.00019352493,0.9743946,0.000010005126,0.000032341293,0.00065436494,0.00017758593,0.0011260717,0.022347143,0.00019817945,0.00084711815,0.00000728355],"about_ca_topic_score_codex":0.0027791192,"about_ca_topic_score_gemma":0.0049472884,"teacher_disagreement_score":0.0027791192,"about_ca_system_score_codex":0.00028850685,"about_ca_system_score_gemma":0.000103990766,"threshold_uncertainty_score":0.005525887},"labels":[],"label_agreement":null},{"id":"W2057078728","doi":"10.1086/430372","title":"Simulations of Stellar Collisions Involving Pre–Main‐Sequence Stars","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Stars; Stellar collision; Smoothed-particle hydrodynamics; Main sequence; Collision; Sequence (biology); Range (aeronautics); Impact parameter","score_opus":0.019897633258585713,"score_gpt":0.2591908201893744,"score_spread":0.2392931869307887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057078728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9899852,0.00016998939,0.004576265,0.000157678,0.000055537363,0.00005984046,0.0005827461,0.00018614231,0.004226499],"genre_scores_gemma":[0.9932955,0.00012776174,0.003985201,0.000082362465,0.000020877946,0.00006009491,0.0010819627,0.00006476453,0.001281575],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997696,0.000048993024,0.000012964562,0.00003052307,0.00007013284,0.0000677348],"domain_scores_gemma":[0.9980877,0.0010448701,0.00016778192,0.00009327478,0.00026899882,0.00033735062],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005414914,0.0005344791,0.0008619292,0.0004875754,0.00077582523,0.00067568023,0.0015448807,0.0010789272,0.0027158894],"category_scores_gemma":[0.002588569,0.00052626035,0.00075094565,0.0007347475,0.00082834595,0.00069086795,0.0007950781,0.0014013668,0.00023880045],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033425863,0.00015435567,0.009249479,0.000046881203,0.00010732084,0.00016315964,0.000138112,0.9837568,0.0016318655,0.0022056631,0.0005519922,0.0016602721],"study_design_scores_gemma":[0.000093378316,0.00009096952,0.0020863486,0.0000060716056,0.000015997359,0.000028252894,0.00006202743,0.99535036,0.0009528567,0.00080426346,0.0004970303,0.000012474377],"about_ca_topic_score_codex":0.019264767,"about_ca_topic_score_gemma":0.013411608,"teacher_disagreement_score":0.019264767,"about_ca_system_score_codex":0.0011554109,"about_ca_system_score_gemma":0.001095678,"threshold_uncertainty_score":0.038305223},"labels":[],"label_agreement":null},{"id":"W2057089429","doi":"10.1086/426077","title":"Differential Imaging with a Multicolor Detector Assembly: A New Exoplanet Finder Concept","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced optical system design","field":"Engineering","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Detector; Strehl ratio; Microlens; Exoplanet; Speckle pattern; Noise (video); Differential (mechanical device); Adaptive optics; Speckle noise","score_opus":0.0067952856265327865,"score_gpt":0.2013062725385718,"score_spread":0.19451098691203902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057089429","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2836957,0.0036590458,0.69306374,0.0012607088,0.0007167286,0.00032013076,0.00027692976,0.0037320135,0.013274966],"genre_scores_gemma":[0.35599118,0.00057657214,0.63171136,0.00035717752,0.00014548791,0.00012756429,0.00017122763,0.00010124731,0.010818185],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99937916,0.0000418709,0.000020258007,0.00015649587,0.0003519982,0.00005015139],"domain_scores_gemma":[0.99948275,0.00008082285,0.00008947759,0.00009244478,0.00015603978,0.000098426106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046055586,0.00033332995,0.0004767985,0.0006224799,0.00049562287,0.0009228838,0.0017730531,0.0008581729,0.0012048658],"category_scores_gemma":[0.0005273193,0.00066667626,0.00030538504,0.00025363304,0.0004937492,0.0011888099,0.00081134046,0.00086517393,0.00067916134],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001487939,0.00012639517,0.0013229303,0.00014445123,0.000018092715,0.00016805735,0.00021002904,0.00071839587,0.9331697,0.011890204,0.0012256283,0.050857242],"study_design_scores_gemma":[0.000060727292,0.000947275,0.0031197222,0.000028179527,0.00004564372,0.0032671,0.000061702085,0.040259477,0.8799343,0.0014752547,0.07070001,0.00010063606],"about_ca_topic_score_codex":0.0002676956,"about_ca_topic_score_gemma":0.00046632322,"teacher_disagreement_score":0.0017730531,"about_ca_system_score_codex":0.00047803356,"about_ca_system_score_gemma":0.0003410633,"threshold_uncertainty_score":0.0040307045},"labels":[],"label_agreement":null},{"id":"W2057129066","doi":"10.1088/0004-637x/778/1/36","title":"DISCOVERY OF A VISUAL T-DWARF TRIPLE SYSTEM AND BINARITY AT THE L/T TRANSITION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Photometry (optics); Spectroscopy; Stellar classification; Binary number; Brown dwarf; Spectral properties; Transition (genetics); Triple system","score_opus":0.0075589622569174186,"score_gpt":0.214143219873274,"score_spread":0.2065842576163566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057129066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979911,0.0000735349,0.0009527774,0.000025740119,0.000003858925,0.0000033568704,0.00007643678,0.00006250672,0.00081077876],"genre_scores_gemma":[0.99863344,0.000014588948,0.0010301727,0.000019722174,0.0000042483844,0.000001984338,0.00009831143,0.000009215773,0.00018836779],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992824,0.0000035805554,0.0000033476067,0.000029269342,0.000015585681,0.000019956493],"domain_scores_gemma":[0.9997538,0.000019366327,0.00006990329,0.00002469396,0.000031817537,0.000100354206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000096531054,0.000107495944,0.00014888107,0.0005803417,0.00036645395,0.0004750476,0.00020892292,0.00030940553,0.0008074617],"category_scores_gemma":[0.00021316073,0.00014354757,0.00013136432,0.00021267575,0.00027303983,0.00018085091,0.0004353153,0.00034100722,0.0003330863],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000473422,0.000074322816,0.37368095,0.000060453473,0.00005372271,0.002466097,0.00071466045,0.00043185533,0.5961133,0.00070979545,0.0007772106,0.02444415],"study_design_scores_gemma":[0.00001781398,0.00023666007,0.9507612,0.0000128322135,0.000035285007,0.007143964,0.0004378331,0.003954566,0.034791667,0.00062367745,0.001958773,0.000025765255],"about_ca_topic_score_codex":0.0014631107,"about_ca_topic_score_gemma":0.0026802705,"teacher_disagreement_score":0.0014631107,"about_ca_system_score_codex":0.00014886304,"about_ca_system_score_gemma":0.00008721144,"threshold_uncertainty_score":0.0029091835},"labels":[],"label_agreement":null},{"id":"W2057148901","doi":"10.1088/0004-637x/737/2/59","title":"SCALING RELATIONS AND OVERABUNDANCE OF MASSIVE CLUSTERS AT<i>z</i>≳ 1 FROM WEAK-LENSING STUDIES WITH THE<i>HUBBLE SPACE TELESCOPE</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":128,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Weak gravitational lensing; Redshift; Strong gravitational lensing; Hubble space telescope; Gravitational lens; Observable; Gravitational lensing formalism; Normalization (sociology); Lambda; Scaling; Hubble's law; Galaxy; Quantum mechanics","score_opus":0.01265718950243701,"score_gpt":0.207794887420484,"score_spread":0.19513769791804697,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057148901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947286,0.00066217215,0.0002484864,0.00035672702,0.000012663472,0.0000061756996,0.0007581259,0.00003487838,0.0031920546],"genre_scores_gemma":[0.9987639,0.00016099618,0.00011680005,0.000032957974,0.000014524686,0.0000033000795,0.000556369,0.000010673899,0.00034053274],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997428,0.00003612839,0.000018822446,0.000092306895,0.000053903685,0.00005610273],"domain_scores_gemma":[0.9945667,0.0009079424,0.0022009204,0.0005705395,0.0006399652,0.001113848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058997556,0.00021602563,0.00019132053,0.0038428616,0.0007452062,0.0014215473,0.00041802487,0.00038361055,0.004339443],"category_scores_gemma":[0.0059189084,0.00019703861,0.00025595006,0.0020791474,0.00083415303,0.00072474696,0.0012651683,0.00038264866,0.00055475347],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011363721,0.000018583061,0.9834314,0.000026175094,0.000051835934,0.00013003309,0.0009324139,0.00024188009,0.0020926,0.0012666174,0.0013990485,0.010295848],"study_design_scores_gemma":[0.000002441608,0.0000080439295,0.9970498,0.000008678645,0.000019693605,0.000103783794,0.00054566824,0.00027638488,0.00013465747,0.0010045869,0.00083980896,0.0000063950283],"about_ca_topic_score_codex":0.022998013,"about_ca_topic_score_gemma":0.025304817,"teacher_disagreement_score":0.022998013,"about_ca_system_score_codex":0.0006426552,"about_ca_system_score_gemma":0.000385502,"threshold_uncertainty_score":0.045728266},"labels":[],"label_agreement":null},{"id":"W2057154619","doi":"10.1086/529120","title":"The Distance and Age of the Supernova Remnants Kes 73 and AXP 1E 1841‐045","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Astrophysics; Physics; Supernova remnant; Pulsar; Supernova; Spectral line; Luminosity; Absorption (acoustics); Line (geometry); Absorption spectroscopy; Astronomy; Geometry; Galaxy; Mathematics; Optics","score_opus":0.008663523366106752,"score_gpt":0.2021763599935173,"score_spread":0.19351283662741053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057154619","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99758184,0.00034509855,0.00016185432,0.000016602846,0.0000064018586,0.000002359649,0.00017953884,0.000010275461,0.0016959357],"genre_scores_gemma":[0.99814236,0.00022093028,0.00027169863,0.000007451613,0.000007177616,0.0000027305089,0.0007607074,0.00000606069,0.00058085716],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998956,0.000007599925,0.000008528633,0.00003427664,0.000028445345,0.000025462374],"domain_scores_gemma":[0.9996076,0.000036340778,0.00017649411,0.000029892766,0.000059847516,0.00008985856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026965907,0.00017089021,0.00019574711,0.0009143296,0.0003984662,0.0006519479,0.00026848796,0.00016344382,0.0015222671],"category_scores_gemma":[0.0005657441,0.00011624843,0.0001951593,0.00043882758,0.00028248885,0.00033883663,0.00060619006,0.00020744906,0.00066653173],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028718016,0.000020931779,0.9757741,0.000027175503,0.00006118053,0.0005592816,0.00026783862,0.00060508447,0.0065030353,0.000525095,0.00037218584,0.014996737],"study_design_scores_gemma":[0.0000027800002,0.000041441384,0.99639577,0.0000050914764,0.000013520958,0.00065701676,0.00013303803,0.0002350209,0.00066852936,0.00007258125,0.0017701243,0.0000049951796],"about_ca_topic_score_codex":0.006106955,"about_ca_topic_score_gemma":0.005241347,"teacher_disagreement_score":0.006106955,"about_ca_system_score_codex":0.00052284816,"about_ca_system_score_gemma":0.00022262639,"threshold_uncertainty_score":0.012142777},"labels":[],"label_agreement":null},{"id":"W2057159274","doi":"10.1086/498092","title":"Discovery of Outlying High‐Velocity Oxygen‐Rich Ejecta in Cassiopeia A","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Ejecta; Cassiopeia A; Physics; Astrophysics; Supernova remnant; Supernova; Population; Knot (papermaking); Astronomy; Geology; Materials science","score_opus":0.007501830018385016,"score_gpt":0.21439565600622146,"score_spread":0.20689382598783645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057159274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99932563,0.00004604077,0.00011743531,0.000008419832,0.0000011504765,0.000003412926,0.00010802358,0.000014054824,0.0003757883],"genre_scores_gemma":[0.99880147,0.00007585353,0.00040192791,0.000009701004,0.000004405275,0.000005171437,0.00054284517,0.000009362941,0.00014922101],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998951,0.000004900097,0.0000054815455,0.00004527847,0.000024768566,0.000024391844],"domain_scores_gemma":[0.9993981,0.00007971877,0.00024484537,0.00008296773,0.000052925727,0.0001414236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018131227,0.00026216032,0.00024359884,0.0011843257,0.0006829691,0.0007684108,0.00030607643,0.0003427676,0.00047940618],"category_scores_gemma":[0.00063760614,0.0002730393,0.0002697686,0.00072679046,0.00046855045,0.0002730971,0.00092933315,0.0003932778,0.00011885947],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034663657,0.000040603198,0.86212224,0.00005958927,0.00017433257,0.0032595433,0.0013506323,0.0007399467,0.12469502,0.00032239995,0.0003234563,0.006565535],"study_design_scores_gemma":[0.000004489243,0.000017741202,0.9976979,0.0000049098144,0.000016345943,0.00036737777,0.00007633959,0.00029125583,0.0010654767,0.000020989726,0.00043341712,0.0000036748936],"about_ca_topic_score_codex":0.009555147,"about_ca_topic_score_gemma":0.015231126,"teacher_disagreement_score":0.009555147,"about_ca_system_score_codex":0.00034187065,"about_ca_system_score_gemma":0.00023481052,"threshold_uncertainty_score":0.0189991},"labels":[],"label_agreement":null},{"id":"W2057351095","doi":"10.1086/518642","title":"Observational Constraints on the Nature of Dark Energy: First Cosmological Results from the ESSENCE Supernova Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":921,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; European Southern Observatory; National Research Council Canada; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Smithsonian Astrophysical Observatory; Consejo Nacional de Investigaciones Científicas y Técnicas; University of Arizona; Australian Research Council; Smithsonian Institution; National Science Foundation","keywords":"Physics; Dark energy; Supernova; Astrophysics; Redshift; Baryon acoustic oscillations; Galaxy; Equation of state; Cosmological constant; Cosmology; Baryon; Astronomy; Theoretical physics; Quantum mechanics","score_opus":0.034163521265068636,"score_gpt":0.2552654481758769,"score_spread":0.22110192691080824,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057351095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99114436,0.0004910716,0.0028328407,0.00006560585,0.0000044924877,0.000009165768,0.0020331615,0.000058737627,0.0033605236],"genre_scores_gemma":[0.99308443,0.00039862908,0.0022469691,0.000030662264,0.0000126776995,0.000005254688,0.003925552,0.000039200735,0.00025664901],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994343,0.00013187586,0.000056817258,0.00008931861,0.00021135413,0.00007635527],"domain_scores_gemma":[0.99569327,0.0014043538,0.0010184973,0.00094941084,0.0004491809,0.00048530396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001771382,0.0005885072,0.00056175096,0.0020567256,0.00042377063,0.0012239721,0.00045440622,0.00026252776,0.0010599586],"category_scores_gemma":[0.005054938,0.0003518471,0.0009554537,0.0014821761,0.00046461413,0.00053551863,0.0014731284,0.00040508865,0.00024364436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023192681,0.000058375248,0.95444745,0.00009254914,0.00039010937,0.00015387898,0.0003140598,0.0151261985,0.005665582,0.004571721,0.0011047154,0.017843513],"study_design_scores_gemma":[0.000051878666,0.00010218551,0.9687778,0.00005363677,0.00021183933,0.00023154772,0.00019748668,0.016329745,0.00545273,0.0032483519,0.0052857334,0.00005720374],"about_ca_topic_score_codex":0.015665663,"about_ca_topic_score_gemma":0.023518989,"teacher_disagreement_score":0.015665663,"about_ca_system_score_codex":0.00050688034,"about_ca_system_score_gemma":0.00041402492,"threshold_uncertainty_score":0.03114891},"labels":[],"label_agreement":null},{"id":"W2057356926","doi":"10.1086/339053","title":"Hot Accretion onto White Dwarfs in Quiescent Dwarf Novae","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"White dwarf; Astrophysics; Physics; Dwarf nova; Accretion (finance); Cataclysmic variable star; Astronomy; Intermediate polar; Stars","score_opus":0.019710648946463762,"score_gpt":0.2306922867378615,"score_spread":0.21098163779139772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057356926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9824363,0.00013284363,0.014960482,0.000103964434,0.000017240834,0.000033728822,0.00007218176,0.000051870276,0.0021913422],"genre_scores_gemma":[0.99305046,0.00007268305,0.005712245,0.00004296106,0.000030164449,0.000029753204,0.000121840356,0.000020963022,0.0009190263],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999074,0.000027418027,0.000007765618,0.000013851648,0.000017619894,0.000025932983],"domain_scores_gemma":[0.9996606,0.0000891067,0.00009725608,0.000024439209,0.000029027675,0.00009949657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043747138,0.00051106664,0.00065526715,0.0005640889,0.00084313954,0.0011545345,0.0008015923,0.00089241914,0.00093034084],"category_scores_gemma":[0.0023225339,0.00070934684,0.0004801427,0.00020620982,0.00092545064,0.00046739305,0.0011599195,0.00032038105,0.0001225905],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005296796,0.00015710427,0.06783378,0.00010319562,0.0002125637,0.0037014766,0.00055999315,0.8785095,0.010676455,0.024826331,0.00069223554,0.012197681],"study_design_scores_gemma":[0.0002915159,0.00014019551,0.015531095,0.000017394788,0.00004225654,0.0002921385,0.00035385712,0.968813,0.0017820266,0.011465866,0.0012392114,0.000031484797],"about_ca_topic_score_codex":0.0078102774,"about_ca_topic_score_gemma":0.007836598,"teacher_disagreement_score":0.0078102774,"about_ca_system_score_codex":0.00068363,"about_ca_system_score_gemma":0.0005820248,"threshold_uncertainty_score":0.015529633},"labels":[],"label_agreement":null},{"id":"W2057359289","doi":"10.1088/0004-637x/772/1/25","title":"THE ATACAMA COSMOLOGY TELESCOPE: DYNAMICAL MASSES AND SCALING RELATIONS FOR A SAMPLE OF MASSIVE SUNYAEV-ZEL'DOVICH EFFECT SELECTED GALAXY CLUSTERS $^,$","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Scaling; Redshift; Cosmology; Galaxy cluster; Galaxy; Amplitude; Sky; Observable; Velocity dispersion","score_opus":0.004549001709478184,"score_gpt":0.21574064863121245,"score_spread":0.21119164692173426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057359289","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99729806,0.0000800057,0.0007624641,0.000035772337,0.0000017326628,0.000011163268,0.0011288112,0.000013624693,0.00066836976],"genre_scores_gemma":[0.9954928,0.000040361097,0.0014624186,0.000009121899,0.000007875494,0.000010873323,0.002807343,0.0000074152877,0.00016173224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997496,0.000042637792,0.00001533101,0.000080205966,0.000076912664,0.000035320438],"domain_scores_gemma":[0.9988636,0.00019843716,0.0003875175,0.00021045808,0.000118505566,0.00022163521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006747507,0.00022635687,0.00023971748,0.0015119833,0.00049734977,0.00069649576,0.00046448637,0.00020812922,0.0011141681],"category_scores_gemma":[0.0024278897,0.00021793616,0.00017311508,0.0011993884,0.00032714236,0.00035972687,0.00082702446,0.000266211,0.00018233166],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011582827,0.000026497797,0.9864601,0.00001746287,0.0000804376,0.00006928034,0.00032166357,0.0017176985,0.0037654983,0.0008376097,0.00070235645,0.0058855754],"study_design_scores_gemma":[0.000008401309,0.000009839584,0.9933536,0.0000021859307,0.0000072222556,0.000046561487,0.000048127047,0.005326074,0.00042706856,0.0001721968,0.00059399195,0.000004819647],"about_ca_topic_score_codex":0.019521173,"about_ca_topic_score_gemma":0.02418555,"teacher_disagreement_score":0.019521173,"about_ca_system_score_codex":0.0006440022,"about_ca_system_score_gemma":0.00028010522,"threshold_uncertainty_score":0.03881508},"labels":[],"label_agreement":null},{"id":"W2057422331","doi":"10.1086/505388","title":"A Fundamental Relation between Compact Stellar Nuclei, Supermassive Black Holes, and Their Host Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":374,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Virgo Cluster; Galaxy; Supermassive black hole; Elliptical galaxy; Hubble space telescope; Galaxy cluster; Hubble sequence; Luminous infrared galaxy; Peculiar galaxy; Galaxy group","score_opus":0.008669100240109535,"score_gpt":0.20334723661822188,"score_spread":0.19467813637811235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057422331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97925574,0.0041181827,0.006530768,0.00057774235,0.000035749155,0.000030223418,0.00044166108,0.0000668555,0.008943117],"genre_scores_gemma":[0.9963464,0.0009246506,0.0014955294,0.00010392166,0.00013191073,0.000012391022,0.00024220739,0.000006970555,0.0007359327],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997427,0.000047645466,0.000019019975,0.000095802345,0.000062177154,0.00003253436],"domain_scores_gemma":[0.995255,0.0016638121,0.002165601,0.00032946258,0.00018797885,0.00039822079],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046732335,0.00022130959,0.00021696318,0.0010663129,0.00036273978,0.0014317599,0.0004998811,0.00077914516,0.0032971778],"category_scores_gemma":[0.0041291537,0.00027915105,0.00012067091,0.001166508,0.0014243699,0.0015796504,0.0007105742,0.00049783284,0.00053786946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007808229,0.00008931533,0.9468019,0.0000919399,0.00004893362,0.00018084586,0.00034037794,0.0006864531,0.010835789,0.022931676,0.00038503535,0.017529694],"study_design_scores_gemma":[0.0000103399625,0.00011031944,0.9770389,0.00002132776,0.00001737303,0.0008078015,0.00017667841,0.0010807441,0.0010273386,0.018129846,0.0015677656,0.000011615769],"about_ca_topic_score_codex":0.0007922529,"about_ca_topic_score_gemma":0.001080187,"teacher_disagreement_score":0.0032971778,"about_ca_system_score_codex":0.00031968296,"about_ca_system_score_gemma":0.00022359964,"threshold_uncertainty_score":0.011030138},"labels":[],"label_agreement":null},{"id":"W2057427832","doi":"10.1088/0004-637x/739/1/36","title":"PLANETESIMALS IN DEBRIS DISKS OF SUN-LIKE STARS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Debris; Stars; Debris disk; Planet; Streaming instability","score_opus":0.01879321952926015,"score_gpt":0.21454815586039502,"score_spread":0.1957549363311349,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057427832","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994388,0.0001810257,0.000070590264,0.000008597129,0.0000011395217,0.00000130444,0.000044640918,0.0000034699585,0.00025031317],"genre_scores_gemma":[0.99963963,0.000094926894,0.000079697515,0.0000036844692,0.0000025245124,0.0000012727503,0.00010357428,9.65249e-7,0.00007377926],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990714,0.000013847286,0.000009263582,0.000035358695,0.00001802537,0.00001632577],"domain_scores_gemma":[0.9994647,0.00011794711,0.00022123415,0.000037675585,0.000047232792,0.000111286914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023573113,0.0001287968,0.00017596138,0.0010841814,0.0005529412,0.00054967694,0.00018273824,0.0002667641,0.0007487097],"category_scores_gemma":[0.001229084,0.00014837539,0.0001344645,0.0005364942,0.00043215358,0.00039926218,0.0004144678,0.0001128133,0.00020070636],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016736517,0.000023787692,0.97897357,0.000036761143,0.000030021061,0.00044620922,0.0005832367,0.00038503038,0.014569005,0.00030034565,0.0000782812,0.004406351],"study_design_scores_gemma":[0.00000444931,0.00003645239,0.99693584,0.0000033651131,0.000009044672,0.00060742785,0.00020092842,0.00045292897,0.0010052555,0.00037022604,0.00037133406,0.0000027081796],"about_ca_topic_score_codex":0.0012608664,"about_ca_topic_score_gemma":0.0013349049,"teacher_disagreement_score":0.0012608664,"about_ca_system_score_codex":0.00027065122,"about_ca_system_score_gemma":0.00008569514,"threshold_uncertainty_score":0.0025070906},"labels":[],"label_agreement":null},{"id":"W2057429525","doi":"10.1086/309035","title":"Probing the Magnetic Field with Molecular Ion Spectra. II.","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Spectral line; Ion; Molecular cloud; Line (geometry); Magnetic field; Astrophysics; Physics; Field (mathematics); Atomic physics; Astronomy; Stars","score_opus":0.004170793754555943,"score_gpt":0.1981059029221657,"score_spread":0.19393510916760975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057429525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98534137,0.0012868252,0.005389879,0.00008362689,0.00004400226,0.00004500203,0.0010506923,0.00012770406,0.006630888],"genre_scores_gemma":[0.9902975,0.0003559378,0.007314373,0.00011993516,0.000035859623,0.000020528096,0.00064013776,0.000019495275,0.0011962372],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998878,0.000010218286,0.0000057732104,0.000038936018,0.000023849823,0.000033441676],"domain_scores_gemma":[0.9997924,0.00003510819,0.00007016046,0.000026807047,0.000033704055,0.000041798863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014999894,0.00019380434,0.00013585901,0.0009458839,0.00031802926,0.00047227353,0.00031378126,0.0003737263,0.003170266],"category_scores_gemma":[0.00030359274,0.00012107226,0.00011959117,0.00049104786,0.00021168301,0.00029969547,0.00035563757,0.00026831345,0.00088946836],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029867544,0.000064443084,0.08796987,0.00010726097,0.000030843938,0.00023125234,0.00007480877,0.00011014251,0.8961461,0.0004948514,0.00033205803,0.014139651],"study_design_scores_gemma":[0.000052744635,0.00049083884,0.5615447,0.000032519238,0.000108195556,0.0029864823,0.00023141813,0.0033490711,0.42000756,0.0013338771,0.009827325,0.00003527359],"about_ca_topic_score_codex":0.0005941225,"about_ca_topic_score_gemma":0.0010007041,"teacher_disagreement_score":0.003170266,"about_ca_system_score_codex":0.00011775166,"about_ca_system_score_gemma":0.00007347073,"threshold_uncertainty_score":0.010605574},"labels":[],"label_agreement":null},{"id":"W2057444928","doi":"10.1086/345597","title":"The Universality of Turbulence in the Molecular Interstellar Medium and Its Exploitation as a Distance Estimator","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Molecular cloud; Astrophysics; Principal component analysis; Calibration; Estimator; Wavelength; Millimeter; Line (geometry); Galaxy; Computational physics; Optics; Statistics; Geometry; Stars; Mathematics","score_opus":0.008221682454824502,"score_gpt":0.23954961993876084,"score_spread":0.23132793748393635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057444928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6795279,0.008301281,0.26906016,0.01001256,0.001962735,0.00004826258,0.0004045314,0.0005830399,0.030099561],"genre_scores_gemma":[0.98140895,0.0015321211,0.01081227,0.00016969128,0.00090593816,0.000011071753,0.0000995714,0.000066067245,0.00499423],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99952507,0.00015663667,0.00003144701,0.00013461818,0.00010821012,0.00004408784],"domain_scores_gemma":[0.9921015,0.003349254,0.0012998194,0.0011327068,0.0015655955,0.00055114133],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014464911,0.00020342406,0.00041332596,0.0010238966,0.00060213025,0.0017670424,0.0006725333,0.0010562415,0.002076623],"category_scores_gemma":[0.01952461,0.0002356747,0.00026144294,0.0006549144,0.0023251993,0.0035824094,0.0011150817,0.00090469804,0.00043881836],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019645097,0.00004516291,0.04324216,0.00039696996,0.00008014411,0.00064395147,0.0007128671,0.017385501,0.014192773,0.77003986,0.008350313,0.14471379],"study_design_scores_gemma":[0.000049176884,0.00024054818,0.0643853,0.00017966433,0.00008269396,0.0019425254,0.0006778179,0.25049162,0.01452479,0.6398926,0.027276631,0.0002567432],"about_ca_topic_score_codex":0.000624762,"about_ca_topic_score_gemma":0.0004950626,"teacher_disagreement_score":0.002076623,"about_ca_system_score_codex":0.0003863655,"about_ca_system_score_gemma":0.0005195581,"threshold_uncertainty_score":0.007649839},"labels":[],"label_agreement":null},{"id":"W2057496128","doi":"10.1088/0004-637x/723/2/1038","title":"THE PHOTOMETRIC PROPERTIES OF A VAST STELLAR SUBSTRUCTURE IN THE OUTSKIRTS OF M33","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Queen's University; University of Toronto; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Surface brightness; Astronomy; Dwarf galaxy; Galaxy; Metallicity; Population; Stellar population; Star formation","score_opus":0.0073707428324448375,"score_gpt":0.19827792891728946,"score_spread":0.1909071860848446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057496128","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938047,0.00003729137,0.00005566687,0.000005943068,4.5761723e-7,0.0000020175428,0.00015714813,0.000004910427,0.00035605417],"genre_scores_gemma":[0.99895966,0.000060620354,0.00022306183,0.000009491105,0.000002370885,0.0000026099817,0.00051884825,0.0000058096634,0.00021757027],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998679,0.000017835546,0.0000052250257,0.000038800204,0.000027171563,0.00004306788],"domain_scores_gemma":[0.99973935,0.00002161133,0.00008143495,0.00004674498,0.000045404417,0.00006548389],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013334102,0.00025919086,0.00027147977,0.0010283147,0.00056634593,0.00035110657,0.00020301773,0.00016214781,0.0010124809],"category_scores_gemma":[0.0003539412,0.00021660393,0.00017001404,0.0013722015,0.00028098142,0.00018620463,0.00050123665,0.00021408833,0.00043598015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000068187146,0.000024875271,0.9704871,0.000017728236,0.00001737669,0.00015383233,0.0018206239,0.00013517919,0.01892089,0.00005847895,0.00021361334,0.008082156],"study_design_scores_gemma":[7.981287e-7,0.000012057804,0.99922085,0.000002319695,0.000003881455,0.00006352723,0.00017399664,0.00004155983,0.00017599932,0.000004528085,0.00029905478,0.0000012585219],"about_ca_topic_score_codex":0.035924368,"about_ca_topic_score_gemma":0.10254571,"teacher_disagreement_score":0.035924368,"about_ca_system_score_codex":0.000323546,"about_ca_system_score_gemma":0.00019162946,"threshold_uncertainty_score":0.071430564},"labels":[],"label_agreement":null},{"id":"W2057614310","doi":"10.1086/511524","title":"The Bulge-Halo Connection in Galaxies: A Physical Interpretation of the <i>V</i> <sub> <i>c</i> </sub> -σ <sub>0</sub> Relation","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Galaxy; Dark matter; Dwarf galaxy; Scaling; Lenticular galaxy; Elliptical galaxy; Galaxy formation and evolution; Correlation function (quantum field theory); Connection (principal bundle)","score_opus":0.004295795345300483,"score_gpt":0.2013697775743554,"score_spread":0.19707398222905492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057614310","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98790306,0.0009165512,0.003991021,0.00043880317,0.000008288049,0.0000056849826,0.000086783446,0.000056235778,0.006593576],"genre_scores_gemma":[0.99920374,0.00012870443,0.00044620692,0.00002098387,0.0000119737415,0.0000021119574,0.00001912324,0.0000038704766,0.00016316645],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999156,0.000023512943,0.000004370205,0.000023463394,0.000015612055,0.000017364096],"domain_scores_gemma":[0.99928683,0.00026574652,0.00022714275,0.000087999884,0.00004563772,0.000086633096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025800936,0.00019616731,0.00012719262,0.0009697996,0.00032936773,0.0014418522,0.0005162696,0.00048763189,0.0020810459],"category_scores_gemma":[0.0018919358,0.00018362902,0.00017677531,0.0009446826,0.0013809963,0.00094477745,0.0009118927,0.00041861428,0.00015217457],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000251105,0.00011691496,0.7685907,0.00015256384,0.00012213129,0.0006939854,0.0030543292,0.01081722,0.029190972,0.13685946,0.0009027172,0.049247827],"study_design_scores_gemma":[0.000024438541,0.000108435706,0.912672,0.00003573433,0.00007274304,0.0009772336,0.00096867076,0.017558018,0.0022859538,0.06184615,0.0034190582,0.000031701948],"about_ca_topic_score_codex":0.0039473805,"about_ca_topic_score_gemma":0.0040698093,"teacher_disagreement_score":0.0039473805,"about_ca_system_score_codex":0.000451481,"about_ca_system_score_gemma":0.00015408295,"threshold_uncertainty_score":0.007848799},"labels":[],"label_agreement":null},{"id":"W2057723053","doi":"10.1086/507323","title":"Tracing the Dynamical History of the Globular Cluster 47 Tucanae","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Blue straggler; Globular cluster; Stellar collision; Mass segregation; Stars; Cluster (spacecraft); Luminosity; Star cluster","score_opus":0.006044580706732644,"score_gpt":0.18922375793240065,"score_spread":0.183179177225668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057723053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99855024,0.000092120405,0.000111193156,0.00005391363,0.000002102737,0.0000031802626,0.00028582063,0.000015397374,0.0008859539],"genre_scores_gemma":[0.9987074,0.000061924795,0.00025971775,0.000009035995,0.0000022573086,0.000004376044,0.00065715116,0.000005861326,0.0002922785],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998759,0.000011224951,0.0000030043234,0.00003868232,0.00002393026,0.000047238394],"domain_scores_gemma":[0.99957174,0.00008488319,0.0000836696,0.000028731762,0.00010974325,0.000121288445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023802074,0.00018779455,0.00027400392,0.0016505615,0.0012617247,0.0007551584,0.0006636676,0.00044210802,0.00071120594],"category_scores_gemma":[0.0012485374,0.0001519339,0.00019500789,0.0016286805,0.00053859793,0.00035714885,0.0006389536,0.00032027264,0.00011952288],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019430059,0.000044667107,0.93239886,0.00004033532,0.00013050945,0.00030085427,0.0012226941,0.030294431,0.011499272,0.0018683077,0.0017709627,0.020234827],"study_design_scores_gemma":[0.000011633383,0.000029698982,0.94935125,0.00002376664,0.00004182879,0.000072179784,0.0007305036,0.044348896,0.001573957,0.00036982683,0.0034139585,0.000032494656],"about_ca_topic_score_codex":0.50067955,"about_ca_topic_score_gemma":0.4454891,"teacher_disagreement_score":0.50067955,"about_ca_system_score_codex":0.004188174,"about_ca_system_score_gemma":0.0012923583,"threshold_uncertainty_score":0.99553055},"labels":[],"label_agreement":null},{"id":"W2057760660","doi":"10.1086/317273","title":"Tentative Detection of Galaxy Spin Correlations in the Tully Catalog","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Galaxy; Spin (aerodynamics); Weak gravitational lensing; Systematic error; Gravitational lens; Cosmology; Perturbation (astronomy); Gravitation; Instability; Galaxy cluster","score_opus":0.007049329433637458,"score_gpt":0.22252541674261117,"score_spread":0.21547608730897372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057760660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9908529,0.0003104447,0.004457405,0.00016316687,0.00002406,0.00001012802,0.0010010303,0.0002230914,0.002957759],"genre_scores_gemma":[0.9952042,0.000079614576,0.00259231,0.000075319855,0.000030845098,0.00001091817,0.0015989039,0.000024309596,0.00038356954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989009,0.0001396192,0.00008277278,0.00023390066,0.00032107253,0.000321784],"domain_scores_gemma":[0.98667836,0.0028075068,0.0033635474,0.003730454,0.0019230844,0.0014971085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021113015,0.00023375663,0.000461367,0.0033461084,0.0009137971,0.0018955258,0.0007826396,0.00048198318,0.0016546438],"category_scores_gemma":[0.009044125,0.00027805773,0.0002754117,0.0013704442,0.00085002894,0.0010266213,0.0019448791,0.00071227836,0.0006424871],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004297045,0.00007882049,0.9104861,0.000092459646,0.0000774623,0.0003235672,0.0013565521,0.0009838797,0.029632876,0.011981748,0.0025666107,0.041990265],"study_design_scores_gemma":[0.00003499211,0.00014900941,0.9718318,0.00004940649,0.00007968683,0.0005250594,0.00031978288,0.005072808,0.010706513,0.0041514374,0.006991261,0.00008820335],"about_ca_topic_score_codex":0.002727852,"about_ca_topic_score_gemma":0.003918235,"teacher_disagreement_score":0.0033461084,"about_ca_system_score_codex":0.0004669353,"about_ca_system_score_gemma":0.00064361724,"threshold_uncertainty_score":0.011165738},"labels":[],"label_agreement":null},{"id":"W2057771221","doi":"10.1088/0004-637x/693/1/617","title":"THE ELLIPTICITIES OF CLUSTER EARLY-TYPE GALAXIES FROM<i>z</i>∼ 1 TO<i>z</i>∼ 0: NO EVOLUTION IN THE OVERALL DISTRIBUTION OF BULGE-TO-DISK RATIOS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Elliptical galaxy; Galaxy cluster; Brightest cluster galaxy; Galaxy; Luminosity; Galaxy group; Galaxy groups and clusters; Redshift; Cluster (spacecraft)","score_opus":0.005333266083409225,"score_gpt":0.20590422674477507,"score_spread":0.20057096066136584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057771221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986041,0.00006624666,0.00003644406,0.000018559811,8.1488514e-7,0.0000012583101,0.00025875022,0.000009429923,0.0010043492],"genre_scores_gemma":[0.99932647,0.000033732686,0.000024671639,0.000008655052,0.0000024172687,0.0000012006184,0.00034534163,0.000004059916,0.00025351852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999349,0.0000043812224,0.0000025049785,0.000022241918,0.000007591234,0.000028321405],"domain_scores_gemma":[0.9989272,0.0001897135,0.00027616974,0.00008144689,0.00016223884,0.00036334316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018753616,0.0001586633,0.00016734305,0.0013629445,0.00022935554,0.0005605993,0.00028971222,0.00029213974,0.002228462],"category_scores_gemma":[0.0008118396,0.00021256506,0.00017401822,0.00045933897,0.00034284554,0.00035581697,0.00041337957,0.00028259042,0.0004960882],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052018743,0.000019822603,0.9739932,0.000018534018,0.000037810947,0.000044590055,0.00042271425,0.00048374705,0.018559322,0.00024335884,0.000309444,0.0053471825],"study_design_scores_gemma":[0.0000015088423,0.0000055252035,0.999637,8.3052555e-7,0.000003149893,0.000013907777,0.000031864016,0.000059443813,0.00017727564,0.000028178658,0.000040189716,0.0000011748544],"about_ca_topic_score_codex":0.006526449,"about_ca_topic_score_gemma":0.008931059,"teacher_disagreement_score":0.006526449,"about_ca_system_score_codex":0.00046610014,"about_ca_system_score_gemma":0.00014123293,"threshold_uncertainty_score":0.012976885},"labels":[],"label_agreement":null},{"id":"W2057840905","doi":"10.1088/0004-637x/759/1/42","title":"THE LONG-TERM X-RAY VARIABILITY OF BROAD ABSORPTION LINE QUASARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Quasar; Line (geometry); Red shift; Spectral line; Absorption (acoustics); Emission spectrum","score_opus":0.016642317179346663,"score_gpt":0.2580782869325567,"score_spread":0.24143596975321002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057840905","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995586,0.000063621286,0.000078931895,0.0000079004,9.073515e-7,8.802508e-7,0.00008556226,0.0000046290616,0.0001990162],"genre_scores_gemma":[0.9993068,0.00004502969,0.00007320795,0.000008862924,0.0000073657934,0.0000022337117,0.00040988042,0.0000027187914,0.00014391798],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998896,0.000010769269,0.000006914874,0.00003239461,0.000020149655,0.000040113897],"domain_scores_gemma":[0.9989724,0.00018003206,0.00051030074,0.000066298846,0.0000750667,0.00019598023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028160552,0.00019305738,0.00016630656,0.000916294,0.0002251502,0.00054886914,0.00025073814,0.00023395818,0.00062392827],"category_scores_gemma":[0.0006777366,0.00011223025,0.00020162531,0.0006447487,0.000277636,0.00037404534,0.0005120143,0.00028640128,0.00019686304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000076024,0.00003794548,0.98235565,0.0000119299,0.00007367957,0.00024092638,0.00014514175,0.00042321763,0.012533139,0.000074231466,0.00008466777,0.0039435276],"study_design_scores_gemma":[8.0611096e-7,0.000019269986,0.99945813,9.2766703e-7,0.0000068668382,0.00008303319,0.000034515448,0.000150962,0.00014790594,0.000015709884,0.00007998607,0.000001828275],"about_ca_topic_score_codex":0.0017612803,"about_ca_topic_score_gemma":0.0030564927,"teacher_disagreement_score":0.0017612803,"about_ca_system_score_codex":0.00021231834,"about_ca_system_score_gemma":0.00007638582,"threshold_uncertainty_score":0.0035020113},"labels":[],"label_agreement":null},{"id":"W2057880141","doi":"10.1088/0004-637x/711/2/641","title":"THE COLLIMATION AND ENERGETICS OF THE BRIGHTEST<i>SWIFT</i>GAMMA-RAY BURSTS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":148,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Royal Military College of Canada","funders":"Jet Propulsion Laboratory; Space Telescope Science Institute; Harvard University; National Aeronautics and Space Administration; California Institute of Technology; Smithsonian Astrophysical Observatory; Gordon and Betty Moore Foundation; Goddard Space Flight Center; Smithsonian Institution; National Science Foundation","keywords":"Afterglow; Physics; Gamma-ray burst; Astrophysics; Achromatic lens; Light curve; Jet (fluid); Collimated light; Viewing angle; Magnetar; Luminosity; Astronomy; Optics; Galaxy; Neutron star; Laser","score_opus":0.004951941628316101,"score_gpt":0.20637122080433323,"score_spread":0.20141927917601712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057880141","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982936,0.00014419678,0.00022443871,0.000013084998,0.0000021747642,0.000003371979,0.00018099356,0.000021422964,0.0011167707],"genre_scores_gemma":[0.9987325,0.000144827,0.0004052826,0.000016336697,0.000008959876,0.0000040075442,0.0005176122,0.000015891677,0.00015454953],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998652,0.000010496172,0.000019012603,0.000034745735,0.000041581872,0.000028860553],"domain_scores_gemma":[0.99931777,0.000058536123,0.00046386747,0.000055125696,0.00005397221,0.00005069059],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025293152,0.00023265423,0.00019654755,0.0010918628,0.00026119582,0.0008340028,0.0002467426,0.0002129781,0.00058928266],"category_scores_gemma":[0.0005567826,0.00020315559,0.00024824642,0.00070437544,0.00028945738,0.00026274537,0.00036122501,0.0002695755,0.00020425611],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017356906,0.000047298476,0.9177546,0.00005213139,0.00005876906,0.00048515858,0.00031420338,0.001411122,0.06493262,0.0004721364,0.00042649597,0.013872005],"study_design_scores_gemma":[0.0000041533394,0.000023188344,0.99673516,0.000005646376,0.000011010141,0.00031500723,0.00005740714,0.0006166342,0.0018083893,0.0000778655,0.00034004383,0.0000055094797],"about_ca_topic_score_codex":0.0035278648,"about_ca_topic_score_gemma":0.0035031373,"teacher_disagreement_score":0.0035278648,"about_ca_system_score_codex":0.00031180412,"about_ca_system_score_gemma":0.00012363249,"threshold_uncertainty_score":0.007014692},"labels":[],"label_agreement":null},{"id":"W2057951961","doi":"10.1086/426128","title":"A Non‐LTE Line‐Blanketed Model of a Solar‐Type Star","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Spectral line; Astrophysics; Atmospheric models; Ionization; Line (geometry); Thermodynamic equilibrium; Atmosphere (unit); Ion; Astronomy; Thermodynamics; Geometry","score_opus":0.010944773666431276,"score_gpt":0.23467717205141014,"score_spread":0.22373239838497888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2057951961","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.842299,0.00040828311,0.10173616,0.0012966242,0.0001940165,0.00012049057,0.0031574762,0.0012076258,0.049580403],"genre_scores_gemma":[0.980431,0.00015284106,0.008762322,0.00020545821,0.00008280767,0.00011724612,0.000815215,0.00016089993,0.009272159],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984837,0.000039211413,0.0000067953947,0.000048015023,0.000025093725,0.000032382184],"domain_scores_gemma":[0.9996593,0.00008530663,0.000041968076,0.000043363765,0.00007535611,0.0000947663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002579218,0.0006721779,0.0007650564,0.00041815444,0.0010010641,0.0012339266,0.002483909,0.002233323,0.0041482365],"category_scores_gemma":[0.0007652799,0.0006043683,0.0012031111,0.0005038381,0.0009260777,0.0015619032,0.001076695,0.0011032053,0.0008677821],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013013829,0.000053051066,0.0029361749,0.000020003923,0.00003361721,0.00012671042,0.000097757096,0.9853474,0.0015908743,0.0077515272,0.0005168318,0.001395852],"study_design_scores_gemma":[0.00004915573,0.000029089577,0.00076809124,0.00000262026,0.000010904578,0.000025164418,0.00002021212,0.9963397,0.00014450414,0.0020026914,0.00059478916,0.000013160934],"about_ca_topic_score_codex":0.043200813,"about_ca_topic_score_gemma":0.016036022,"teacher_disagreement_score":0.043200813,"about_ca_system_score_codex":0.00129942,"about_ca_system_score_gemma":0.00081263797,"threshold_uncertainty_score":0.08589876},"labels":[],"label_agreement":null},{"id":"W2058101940","doi":"10.1086/339230","title":"The Intrinsic Shapes of Molecular Cloud Fragments over a Range of Length Scales","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Prolate spheroid; Oblate spheroid; Molecular cloud; Range (aeronautics); Physics; Astrophysics; Materials science; Classical mechanics","score_opus":0.009099795432585257,"score_gpt":0.22353532738052392,"score_spread":0.21443553194793866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058101940","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944354,0.00008866589,0.0038150095,0.000014753399,8.739553e-7,0.000004701755,0.00058892556,0.00006127618,0.0009903808],"genre_scores_gemma":[0.99760985,0.00006134728,0.001489948,0.0000036877059,0.0000022049046,0.0000046404857,0.0006842384,0.000024299688,0.000119808064],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988985,0.0000104715555,0.0000049643704,0.000039394083,0.00002968929,0.000025593497],"domain_scores_gemma":[0.9982895,0.00037383777,0.00066143146,0.00022520023,0.00026483196,0.00018520596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025680853,0.00014665192,0.00017628432,0.0009663542,0.0003393115,0.0006020703,0.00025769125,0.0001368487,0.001157079],"category_scores_gemma":[0.0019758719,0.00019648777,0.00029281704,0.0008017321,0.00040129127,0.0007598675,0.00045900434,0.00024064767,0.00025351797],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036746627,0.000030919033,0.86955565,0.00008273359,0.00012343444,0.0001875494,0.00067327684,0.020520313,0.08005955,0.0023806358,0.0002683953,0.025750078],"study_design_scores_gemma":[0.0000051188313,0.00004984511,0.9569666,0.0000062617487,0.000026176627,0.00039426464,0.00015963022,0.03193764,0.00848438,0.0012719659,0.0006752883,0.000022974335],"about_ca_topic_score_codex":0.0026776958,"about_ca_topic_score_gemma":0.0031362965,"teacher_disagreement_score":0.0026776958,"about_ca_system_score_codex":0.00044636108,"about_ca_system_score_gemma":0.00016817871,"threshold_uncertainty_score":0.005324185},"labels":[],"label_agreement":null},{"id":"W2058129926","doi":"10.1086/319730","title":"Evidence of a Supermassive Black Hole in the Galaxy NGC 1023 from the Nuclear Stellar Dynamics","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Supermassive black hole; Galaxy; Black hole (networking); Velocity dispersion; Space Telescope Imaging Spectrograph; Stellar kinematics; Stellar mass; Astronomy; Star formation; Milky Way; Hubble space telescope","score_opus":0.012908308783342167,"score_gpt":0.22251615899339725,"score_spread":0.20960785021005507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058129926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99872845,0.00006134513,0.00054718467,0.000020065023,0.0000012680384,0.000002103995,0.000063881555,0.000028805343,0.000546827],"genre_scores_gemma":[0.9994766,0.000024157085,0.00026918057,0.000007705165,0.000002229218,0.000001220593,0.00015050896,0.0000044856906,0.00006399047],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998977,0.00001658195,0.000006828212,0.000022702956,0.000035773148,0.000020399999],"domain_scores_gemma":[0.9993647,0.000111939735,0.000296118,0.00005721773,0.00004095318,0.00012905114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026486692,0.00036126428,0.0002256826,0.00066678243,0.00025040415,0.00056272116,0.0003539884,0.0003683785,0.0013886569],"category_scores_gemma":[0.0008814126,0.00015400819,0.0003712106,0.00054968457,0.0003894826,0.00027613263,0.00032971048,0.0002092381,0.00033063025],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001522885,0.00003911656,0.9591656,0.000025530599,0.000067336114,0.00079983065,0.00030486516,0.0050213197,0.025938429,0.0011780498,0.00017557126,0.0071321656],"study_design_scores_gemma":[0.000015369576,0.00008465053,0.97201747,0.000012519399,0.00003292542,0.0009436684,0.00017024102,0.02333054,0.0017143255,0.0011214684,0.00054420886,0.000012580392],"about_ca_topic_score_codex":0.0070801247,"about_ca_topic_score_gemma":0.010046955,"teacher_disagreement_score":0.0070801247,"about_ca_system_score_codex":0.0005341916,"about_ca_system_score_gemma":0.00018894313,"threshold_uncertainty_score":0.014077842},"labels":[],"label_agreement":null},{"id":"W2058149148","doi":"10.1088/0004-637x/697/2/1057","title":"UNDERSTANDING COMPACT OBJECT FORMATION AND NATAL KICKS. II. THE CASE OF XTE J1118 + 480","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Black hole (networking); Solar mass; Roche lobe; Metallicity; Astronomy; Binary system; Stellar black hole; Binary number; Binary star; Stars; Galaxy","score_opus":0.039923602299307505,"score_gpt":0.25756097520630566,"score_spread":0.21763737290699817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058149148","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98756856,0.0022347937,0.0024892392,0.00036658722,0.000007667765,0.000011190758,0.0000634385,0.000015072995,0.007243432],"genre_scores_gemma":[0.9979814,0.00067767524,0.0005465897,0.000020058373,0.000012913968,0.0000044728117,0.00007990561,0.0000026525868,0.00067417684],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999497,0.000007885445,0.0000026939324,0.00001321279,0.000007797882,0.00001867951],"domain_scores_gemma":[0.99958557,0.00011549316,0.00020533412,0.0000354809,0.000015982188,0.000042215055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017553658,0.0002532474,0.00023502331,0.0006396201,0.0003271926,0.0013635261,0.00037047878,0.0006786528,0.0019642538],"category_scores_gemma":[0.0015672804,0.00019721416,0.00011797925,0.0004023132,0.00080879463,0.0021188173,0.0007335882,0.00041083855,0.00032125763],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002920887,0.00014296637,0.8021853,0.00028469999,0.00007643912,0.0034031067,0.0024794233,0.0086789075,0.013553552,0.0779846,0.000977915,0.08994106],"study_design_scores_gemma":[0.000015962687,0.00006560142,0.914681,0.00006367568,0.000039948318,0.0020111057,0.0023822836,0.021750554,0.0020671955,0.051347457,0.005551363,0.000023904926],"about_ca_topic_score_codex":0.0027805616,"about_ca_topic_score_gemma":0.0034107685,"teacher_disagreement_score":0.0027805616,"about_ca_system_score_codex":0.00044411508,"about_ca_system_score_gemma":0.00014493354,"threshold_uncertainty_score":0.0065710545},"labels":[],"label_agreement":null},{"id":"W2058152646","doi":"10.1088/0004-637x/772/2/137","title":"<i>HERSCHEL</i>-ATLAS: A BINARY HyLIRG PINPOINTING A CLUSTER OF STARBURSTING PROTOELLIPTICALS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":191,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Star formation; Astronomy; Luminous infrared galaxy; Galaxy cluster; Galaxy formation and evolution; Dark matter; Star cluster","score_opus":0.008272708033382481,"score_gpt":0.2143904725783759,"score_spread":0.20611776454499342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058152646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9284508,0.001844281,0.0033763659,0.0010768432,0.00009784291,0.000081012186,0.019318521,0.0011625773,0.04459179],"genre_scores_gemma":[0.97706884,0.0002231515,0.0047520692,0.00023348548,0.00007372558,0.000017635513,0.01243996,0.00006654088,0.005124637],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999051,0.000006367986,0.0000041261874,0.000028385646,0.00001872905,0.000037188707],"domain_scores_gemma":[0.9998503,0.000008449275,0.000036095076,0.000016021952,0.00002028113,0.00006889376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016549585,0.00018929405,0.00016177518,0.0010346333,0.00049491564,0.000690179,0.000308792,0.00040406393,0.0064039608],"category_scores_gemma":[0.00018857652,0.00008994715,0.00010107441,0.00055092765,0.00029901907,0.0005238081,0.0006849134,0.0002477858,0.0019734127],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015392285,0.00015813732,0.66474104,0.00035132916,0.000091930335,0.0038300015,0.00070190546,0.0012956673,0.16077183,0.015362006,0.06410208,0.08705479],"study_design_scores_gemma":[0.000036889032,0.00013710566,0.9073686,0.000056709854,0.00004461573,0.0032471484,0.00042787803,0.0027153678,0.011826068,0.0019978106,0.072108515,0.000033311273],"about_ca_topic_score_codex":0.0077637606,"about_ca_topic_score_gemma":0.015895534,"teacher_disagreement_score":0.0077637606,"about_ca_system_score_codex":0.00059756625,"about_ca_system_score_gemma":0.00023682756,"threshold_uncertainty_score":0.02142334},"labels":[],"label_agreement":null},{"id":"W2058175432","doi":"10.1086/317017","title":"Normal Coordinate Analysis and Vibrational Spectra of Aromatic Carbon Nanostructures","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Spectral line; Molecule; Physics; Infrared spectroscopy; Hamiltonian (control theory); Molecular physics; Molecular vibration; Infrared; Normal mode; Atomic physics; Dehydrogenation; Chemistry; Vibration; Quantum mechanics; Organic chemistry","score_opus":0.003718681539942478,"score_gpt":0.20458608065898054,"score_spread":0.20086739911903806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058175432","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.977979,0.00016751449,0.014920797,0.000041428913,0.000009265628,0.000008070464,0.00029053396,0.00015986373,0.0064235115],"genre_scores_gemma":[0.9926277,0.000077690376,0.0056123314,0.00000346205,0.0000022488837,0.000009415676,0.00032091216,0.000022218199,0.0013240651],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99995697,0.000004230384,0.0000012593986,0.0000108478,0.000020134627,0.000006462141],"domain_scores_gemma":[0.99994385,0.000015324546,0.000005320061,0.0000072730973,0.000022406475,0.000005718211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000073559066,0.00013454504,0.00010524736,0.00041131725,0.00017825294,0.00013668425,0.00023542205,0.00012617897,0.003138189],"category_scores_gemma":[0.00019023039,0.00005162936,0.00009293398,0.00024730217,0.00013721432,0.000121728284,0.00008189542,0.000111386165,0.00019406265],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016838562,0.000041776693,0.004379985,0.00013534514,0.000017246204,0.0002367556,0.00023741809,0.07998016,0.8627036,0.029529966,0.000907107,0.02166227],"study_design_scores_gemma":[0.00001197849,0.00012425244,0.019522144,0.000008048008,0.000009389666,0.00017969456,0.00012729352,0.75373495,0.2172483,0.0060662013,0.002942141,0.000025527848],"about_ca_topic_score_codex":0.0012543071,"about_ca_topic_score_gemma":0.0008518639,"teacher_disagreement_score":0.003138189,"about_ca_system_score_codex":0.0003147334,"about_ca_system_score_gemma":0.00009065679,"threshold_uncertainty_score":0.010498285},"labels":[],"label_agreement":null},{"id":"W2058197414","doi":"10.1086/341484","title":"Search for Non-Gaussian Signals in the BOOMERANG Maps: Pixel-Space Analysis","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Gaussian; Skewness; Non-Gaussianity; Kurtosis; Cosmic background radiation; Astrophysics; Sky; Anisotropy; Statistics; Mathematics; Optics","score_opus":0.015358035233124174,"score_gpt":0.2753920487398221,"score_spread":0.2600340135066979,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058197414","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9228023,0.000112728376,0.075351246,0.00010253039,0.0000059294753,0.000016164735,0.00021197413,0.0004246072,0.000972452],"genre_scores_gemma":[0.9854956,0.00003722597,0.013720731,0.000018759692,0.000006070277,0.000008981783,0.00043994212,0.00006056217,0.00021192027],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996369,0.000103789556,0.0000115707735,0.000083954015,0.0000925364,0.000071232294],"domain_scores_gemma":[0.9976534,0.0012252857,0.00034636146,0.00030049533,0.00034342983,0.00013106702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012730191,0.00027509863,0.00032453236,0.0011662507,0.0004961203,0.00084531144,0.0004632043,0.00035551368,0.0013896802],"category_scores_gemma":[0.005371332,0.00017194364,0.00040024443,0.001012345,0.00055441144,0.0007209744,0.0005154111,0.00038521292,0.00021623829],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023421887,0.00022638736,0.5647096,0.00019809097,0.0010068846,0.0010405162,0.0013986436,0.17103869,0.043942686,0.064240366,0.0037258586,0.14613008],"study_design_scores_gemma":[0.000055903896,0.00016161123,0.29491606,0.000020937188,0.00013172475,0.0006848574,0.00040371576,0.642974,0.015863603,0.03975,0.0049366127,0.00010104061],"about_ca_topic_score_codex":0.0024863158,"about_ca_topic_score_gemma":0.002948074,"teacher_disagreement_score":0.0024863158,"about_ca_system_score_codex":0.00027437383,"about_ca_system_score_gemma":0.00037020323,"threshold_uncertainty_score":0.006732464},"labels":[],"label_agreement":null},{"id":"W2058380298","doi":"10.1088/0004-637x/743/1/91","title":"RADIATION-HYDRODYNAMIC SIMULATIONS OF PROTOSTELLAR OUTFLOWS: SYNTHETIC OBSERVATIONS AND DATA COMPARISONS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Harvard University; National Science Foundation","keywords":"Physics; Radiation; Astrophysics; Protostar; Astronomy; Star formation; Optics; Stars","score_opus":0.05947036268105692,"score_gpt":0.27942041827753517,"score_spread":0.21995005559647823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058380298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953017,0.00004845649,0.0024829656,0.00008599072,0.000011799254,0.00002242753,0.0005558362,0.0001917665,0.0012991447],"genre_scores_gemma":[0.9960639,0.000030312474,0.0026011346,0.000043577842,0.000008356076,0.00003215239,0.000997961,0.000056026925,0.00016654779],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997334,0.000075060874,0.0000211771,0.000057479418,0.000054366785,0.00005854919],"domain_scores_gemma":[0.9983858,0.00081209984,0.00024759985,0.00014615999,0.00022000489,0.0001882999],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006199571,0.0006896579,0.00063256506,0.00046451937,0.0005138688,0.0006363207,0.0011144769,0.0010281125,0.00069379486],"category_scores_gemma":[0.0025621646,0.00033780886,0.0008366765,0.00063240743,0.00083524786,0.00045992958,0.0005013004,0.00069960346,0.00009180049],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002344907,0.00024333577,0.015416835,0.000032218817,0.00006339885,0.00014453125,0.0001141125,0.97868186,0.0022260197,0.001300581,0.00033529807,0.0012074213],"study_design_scores_gemma":[0.00010201638,0.000053463235,0.0038198433,0.0000044857507,0.000010459215,0.000023659592,0.000039763407,0.99430484,0.0010295138,0.0004401662,0.0001593705,0.000012446926],"about_ca_topic_score_codex":0.012638985,"about_ca_topic_score_gemma":0.0066484367,"teacher_disagreement_score":0.012638985,"about_ca_system_score_codex":0.0010354281,"about_ca_system_score_gemma":0.0005469165,"threshold_uncertainty_score":0.025130808},"labels":[],"label_agreement":null},{"id":"W2058468570","doi":"10.1086/519835","title":"Reconstructing the Thomson Optical Depth due to Patchy Reionization with 21 cm Fluctuation Maps","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University; Canadian Institute for Theoretical Astrophysics; Research Canada","funders":"","keywords":"Reionization; Cosmic microwave background; Physics; Astrophysics; Optical depth; Redshift; Polarization (electrochemistry); COSMIC cancer database; Brightness; Electron; Astronomy; Optics; Anisotropy; Galaxy; Chemistry","score_opus":0.007137869166554261,"score_gpt":0.2379702086296015,"score_spread":0.23083233946304724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058468570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9774565,0.00011084485,0.020917347,0.00003807237,0.000005023849,0.0000054231473,0.00026027346,0.00014120882,0.0010653259],"genre_scores_gemma":[0.99680305,0.000038948492,0.002842811,0.0000042313663,0.0000053529598,0.0000015391021,0.00015272487,0.000018762534,0.00013266345],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999912,0.000013968689,0.00000259254,0.00002376698,0.000022308921,0.000025279463],"domain_scores_gemma":[0.99955696,0.00012245914,0.00011938385,0.000070793794,0.000064581676,0.000065748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023015599,0.00023419989,0.00017946071,0.0008332688,0.00010135555,0.00031496992,0.00024323979,0.00014985897,0.0006402916],"category_scores_gemma":[0.0014501619,0.0001794053,0.00017559231,0.000594521,0.00016360535,0.00038524834,0.00048477188,0.0002079509,0.000111999216],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007610009,0.000073431846,0.38608545,0.00010012124,0.0002752026,0.0012300992,0.00055689504,0.15081659,0.32322136,0.009392215,0.0012415685,0.1262461],"study_design_scores_gemma":[0.000014649856,0.000059088372,0.56432617,0.000009225839,0.000043660755,0.00046496117,0.000104844024,0.4036935,0.02526469,0.0044855927,0.0014820361,0.000051668754],"about_ca_topic_score_codex":0.002531274,"about_ca_topic_score_gemma":0.002897394,"teacher_disagreement_score":0.002531274,"about_ca_system_score_codex":0.00035171548,"about_ca_system_score_gemma":0.00014077847,"threshold_uncertainty_score":0.0050331354},"labels":[],"label_agreement":null},{"id":"W2058505535","doi":"10.1088/0004-637x/775/2/95","title":"A KINEMATIC DISTANCE STUDY OF THE PLANETARY NEBULAE-SUPERNOVA REMNANT-H II REGION COMPLEX AT G35.6–0.5","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Supernova remnant; Planetary nebula; Molecular cloud; Spectral line; Kinematics; Supernova; H II region","score_opus":0.01949633572360019,"score_gpt":0.226923330438696,"score_spread":0.20742699471509582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058505535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988966,0.00007504104,0.0001604195,0.0000066383245,0.0000012502816,0.000002684019,0.00011029257,0.0000061817123,0.0007410351],"genre_scores_gemma":[0.9990415,0.000020804371,0.00040265644,0.0000052676883,0.0000016743322,0.00000107201,0.00035556834,0.0000022585482,0.00016907715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989986,0.000008492786,0.0000073108918,0.000034164263,0.000021338119,0.00002891103],"domain_scores_gemma":[0.9997329,0.000026808266,0.00009156372,0.000015919919,0.000037331214,0.00009547288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001415503,0.00014015658,0.00011280093,0.00073688733,0.00026275287,0.0004103833,0.00022324963,0.00016266598,0.0009441665],"category_scores_gemma":[0.00036240934,0.00008642347,0.0002014443,0.00057221897,0.00017112274,0.00023327881,0.0003600451,0.00014361931,0.00029467663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002170178,0.00004706553,0.9586401,0.000016594699,0.00006196745,0.0006929764,0.00035024717,0.0008807799,0.028804969,0.0008091511,0.00024341492,0.009235694],"study_design_scores_gemma":[0.000004667074,0.00007171209,0.995946,0.0000021605276,0.000015279064,0.00058432075,0.00012985308,0.0010902011,0.0012891169,0.0000914395,0.0007705951,0.000004560526],"about_ca_topic_score_codex":0.009231245,"about_ca_topic_score_gemma":0.011475946,"teacher_disagreement_score":0.009231245,"about_ca_system_score_codex":0.00046220535,"about_ca_system_score_gemma":0.00014447738,"threshold_uncertainty_score":0.018355012},"labels":[],"label_agreement":null},{"id":"W2058565854","doi":"10.1088/0004-637x/798/1/15","title":"EVENT HORIZON TELESCOPE EVIDENCE FOR ALIGNMENT OF THE BLACK HOLE IN THE CENTER OF THE MILKY WAY WITH THE INNER STELLAR DISK","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Black hole (networking); Astrophysics; Event horizon; Milky Way; Astronomy; Stellar black hole; Accretion (finance); Intermediate-mass black hole; Angular momentum; Sky; Galactic Center; Horizon; Binary black hole; Rotating black hole; Telescope; Spin-flip; Galaxy; Classical mechanics; Gravitational wave","score_opus":0.016853036129761058,"score_gpt":0.24396159009953963,"score_spread":0.22710855396977858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058565854","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965823,0.00013921704,0.0004885665,0.00008887765,0.000014476963,0.000004654094,0.00012023609,0.000027474021,0.0025341245],"genre_scores_gemma":[0.9991391,0.000039996954,0.0004550558,0.000027430895,0.000012866905,0.0000020825094,0.00014162163,0.000007951419,0.00017391788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997049,0.000030007533,0.000014910102,0.00007682258,0.00009127658,0.000082078564],"domain_scores_gemma":[0.9984371,0.000118748256,0.00078701833,0.0001637042,0.00020007098,0.00029339566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059831253,0.00017065801,0.00029900396,0.00090980117,0.0004893139,0.0007369288,0.0003909226,0.00052643643,0.0011944495],"category_scores_gemma":[0.0012589667,0.0002513351,0.00020563767,0.0007483549,0.0007256714,0.0005220663,0.0008815553,0.00038660478,0.00030725877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046672038,0.00010138395,0.8574889,0.000057876234,0.00007739601,0.000714393,0.0012676567,0.0002105813,0.12291417,0.0025301708,0.0008729297,0.013297788],"study_design_scores_gemma":[0.0000070607007,0.00002764073,0.9980769,0.0000042735073,0.000009751007,0.00013914594,0.00012312325,0.00013009642,0.00091854896,0.00013953223,0.00042093816,0.000003043856],"about_ca_topic_score_codex":0.0030374902,"about_ca_topic_score_gemma":0.004959075,"teacher_disagreement_score":0.0030374902,"about_ca_system_score_codex":0.00036009465,"about_ca_system_score_gemma":0.0002139824,"threshold_uncertainty_score":0.0060396194},"labels":[],"label_agreement":null},{"id":"W2058594171","doi":"10.1086/522074","title":"Nonlinear Evolution of Hydrodynamical Shear Flows in Two Dimensions","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Instability; Vorticity; Inviscid flow; Rotational symmetry; Angular momentum; Shear flow; Perturbation (astronomy); Vortex; Wavenumber","score_opus":0.006822005088415237,"score_gpt":0.25864639318652216,"score_spread":0.2518243880981069,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058594171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9811156,0.00019111765,0.012028756,0.00037056016,0.00004251369,0.000023614479,0.00008740871,0.00011816387,0.0060222605],"genre_scores_gemma":[0.9930774,0.00013710387,0.004853135,0.000066345965,0.00002155831,0.00001919203,0.000060884915,0.000022591792,0.0017417375],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990404,0.000024743196,0.0000058156274,0.00001609656,0.0000219478,0.000027317868],"domain_scores_gemma":[0.9997036,0.00007187502,0.00009464559,0.000022144292,0.00004079941,0.000067030676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014970459,0.00066342193,0.00026795323,0.000628062,0.000526768,0.0013619129,0.0002979789,0.0008396915,0.00086871244],"category_scores_gemma":[0.0008951102,0.00027471778,0.00041294235,0.00035895896,0.0013513294,0.000987298,0.001060061,0.0006028291,0.000111492445],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055454107,0.00023563544,0.021566162,0.00010600956,0.00016088784,0.0017054144,0.001315223,0.741197,0.12832344,0.09551583,0.0008343676,0.008485538],"study_design_scores_gemma":[0.000044256467,0.000073120595,0.0060198037,0.000008561747,0.000012797578,0.00009133897,0.00012793804,0.9800617,0.0032872309,0.009384051,0.00083322823,0.000055986675],"about_ca_topic_score_codex":0.004932227,"about_ca_topic_score_gemma":0.0018181752,"teacher_disagreement_score":0.004932227,"about_ca_system_score_codex":0.00085500727,"about_ca_system_score_gemma":0.00043214983,"threshold_uncertainty_score":0.00980705},"labels":[],"label_agreement":null},{"id":"W2058622036","doi":"10.1086/320440","title":"Mass‐losing Semiregular Variable Stars in Baade’s Windows","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Stars; Photometry (optics); Asymptotic giant branch; Astronomy; Bulge; Carbon star; Large Magellanic Cloud; Variable star; Light curve","score_opus":0.009590380238856526,"score_gpt":0.21481550616036843,"score_spread":0.2052251259215119,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058622036","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996532,0.000036727895,0.00005334707,0.000003544723,7.19076e-7,0.0000022503305,0.00006267307,0.0000028087504,0.00018469206],"genre_scores_gemma":[0.99932134,0.00004356328,0.00014706451,0.0000033013011,0.0000015755853,0.0000033227639,0.00035835666,0.000002135006,0.000119414115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997526,0.00003015631,0.000014996893,0.00008431615,0.000051417363,0.000066510845],"domain_scores_gemma":[0.9995078,0.000048785096,0.000155335,0.000047326273,0.00006184896,0.000178833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030484397,0.00023624954,0.00037347505,0.0019227865,0.00062949845,0.00078844395,0.00022470391,0.00020897036,0.0005960396],"category_scores_gemma":[0.0006200153,0.00018576307,0.0002466191,0.0012670349,0.00033583658,0.00034614137,0.00081456883,0.00021344304,0.00023119742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013450925,0.000022430098,0.98957574,0.000011644931,0.000038608356,0.0001036909,0.00044069262,0.00013680686,0.0055865264,0.0001528749,0.000053049447,0.0037434285],"study_design_scores_gemma":[0.0000020949938,0.00002754016,0.9988661,0.0000014165195,0.0000066929542,0.0001000251,0.0001430898,0.0001514303,0.00034433077,0.000031471172,0.0003236773,0.0000021192361],"about_ca_topic_score_codex":0.009574142,"about_ca_topic_score_gemma":0.015450462,"teacher_disagreement_score":0.009574142,"about_ca_system_score_codex":0.00033973972,"about_ca_system_score_gemma":0.00023823419,"threshold_uncertainty_score":0.01903683},"labels":[],"label_agreement":null},{"id":"W2058716140","doi":"10.1088/0004-637x/787/2/161","title":"INTERSTELLAR SCINTILLATION OF THE DOUBLE PULSAR J0737–3039","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Pulsar; Astrophysics; Orbit (dynamics); Millisecond pulsar; Orbital inclination; Scintillation; Angular velocity; Astronomy; Classical mechanics; Binary number; Optics","score_opus":0.010891004637088334,"score_gpt":0.2933053509699648,"score_spread":0.2824143463328765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058716140","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974214,0.00035180346,0.00024349085,0.000035949648,0.00002650996,0.000011498693,0.00066402386,0.00004298045,0.001202397],"genre_scores_gemma":[0.9982304,0.00011128302,0.00032597446,0.000022592783,0.00002490808,0.00001254305,0.0010499698,0.000009857141,0.00021253599],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979633,0.000013724763,0.000013437384,0.00005010686,0.00007477943,0.000051630075],"domain_scores_gemma":[0.9994097,0.000055443645,0.0002073783,0.00006932822,0.00012160173,0.00013648171],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027273723,0.0003106419,0.00059538806,0.0013827104,0.0006333001,0.0004498756,0.00032986046,0.00032457942,0.0004944074],"category_scores_gemma":[0.00051803526,0.00014772968,0.0002300825,0.0012965266,0.0003500144,0.00023936052,0.0006061612,0.0005523455,0.00023852942],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00088196597,0.000358856,0.7836104,0.0001763836,0.00036712032,0.0034058755,0.00094278774,0.00221013,0.16625719,0.0006106934,0.004376243,0.036802378],"study_design_scores_gemma":[0.000023127084,0.00017293054,0.98649466,0.000017133403,0.00005247443,0.0011625863,0.00016385512,0.0022544214,0.006054849,0.00012364707,0.0034499422,0.000030499641],"about_ca_topic_score_codex":0.010276422,"about_ca_topic_score_gemma":0.022352183,"teacher_disagreement_score":0.010276422,"about_ca_system_score_codex":0.00063544133,"about_ca_system_score_gemma":0.00042939282,"threshold_uncertainty_score":0.020433247},"labels":[],"label_agreement":null},{"id":"W2058862335","doi":"10.1086/423620","title":"The Very Young Radio Pulsar J1357-6429","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Glitch; Vela; Luminosity; Supernova; Supernova remnant; Neutron star; Binary pulsar","score_opus":0.00879458227342696,"score_gpt":0.2915696923511932,"score_spread":0.28277511007776623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058862335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99723023,0.000613135,0.00028840156,0.00007788627,0.00003066918,0.000006678247,0.00014576585,0.000019710582,0.001587569],"genre_scores_gemma":[0.99813336,0.00023498593,0.00044587516,0.00007738438,0.000028136406,0.0000034988866,0.00040418573,0.0000035214794,0.0006692231],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999033,0.0000063081593,0.0000064229826,0.000022371534,0.000035579684,0.000026090249],"domain_scores_gemma":[0.9997727,0.000014870541,0.00007477368,0.000020097039,0.00002649515,0.00009109311],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015401302,0.0001673986,0.00020690485,0.00043015488,0.00034896718,0.00043674908,0.0003180429,0.00025213792,0.00072243664],"category_scores_gemma":[0.00035450511,0.000082362196,0.000081099155,0.00036935878,0.00028799238,0.00024654128,0.00057092815,0.00022581774,0.0004931796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058783434,0.00018078508,0.6237467,0.00014608065,0.00010858815,0.024267219,0.00084751454,0.0003974483,0.282646,0.0027485031,0.0038507814,0.060472634],"study_design_scores_gemma":[0.00006573014,0.00081150647,0.9009129,0.000032885808,0.000070510745,0.035436615,0.00038351957,0.0006832374,0.015960077,0.0011729785,0.044420976,0.000049007143],"about_ca_topic_score_codex":0.002095125,"about_ca_topic_score_gemma":0.0029381658,"teacher_disagreement_score":0.002095125,"about_ca_system_score_codex":0.00018471005,"about_ca_system_score_gemma":0.00016606443,"threshold_uncertainty_score":0.004165828},"labels":[],"label_agreement":null},{"id":"W2058893304","doi":"10.1088/0004-637x/770/2/93","title":"DISCOVERY OF TeV GAMMA-RAY EMISSION TOWARD SUPERNOVA REMNANT SNR G78.2+2.1","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Supernova remnant; Crab Nebula; Particle acceleration; Observatory; Cosmic ray; Spectral index; Flux (metallurgy); Photon","score_opus":0.009989351801443308,"score_gpt":0.21844435877320506,"score_spread":0.20845500697176175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058893304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988825,0.00011862258,0.00014779724,0.000008755548,0.0000040246164,0.000004108161,0.00011620901,0.000026944022,0.000691159],"genre_scores_gemma":[0.9981146,0.00009623988,0.0005822574,0.000025058025,0.000013804388,0.000006573629,0.00081313145,0.000012173225,0.000336218],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999081,0.0000052292635,0.0000051937377,0.000026603846,0.000031484447,0.000023300128],"domain_scores_gemma":[0.999731,0.000018852294,0.0001145644,0.000039870592,0.000030101413,0.000065597276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017756659,0.00035947832,0.00038260323,0.00051521044,0.00030766972,0.0006218757,0.00038261875,0.00033806724,0.0007134781],"category_scores_gemma":[0.00034677293,0.00015940635,0.00020797271,0.00037131322,0.00027047863,0.00016145232,0.00063549035,0.00022064443,0.00044890874],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093873363,0.00009245417,0.5275503,0.000101985715,0.00013950873,0.008646148,0.0004645832,0.00042380244,0.4451024,0.0004793101,0.0005525656,0.01550825],"study_design_scores_gemma":[0.000037622714,0.0005397725,0.95018744,0.000018137545,0.00012048434,0.010468676,0.00022398216,0.0010893593,0.032127105,0.00024866112,0.004914765,0.000024085333],"about_ca_topic_score_codex":0.001461931,"about_ca_topic_score_gemma":0.0027906175,"teacher_disagreement_score":0.001461931,"about_ca_system_score_codex":0.00020824275,"about_ca_system_score_gemma":0.00011741541,"threshold_uncertainty_score":0.0029067993},"labels":[],"label_agreement":null},{"id":"W2058998647","doi":"10.1088/0004-637x/725/1/922","title":"RADIO AND X-RAY OBSERVATIONS OF THE TYPE Ic SN 2007gr REVEAL AN ORDINARY, NON-RELATIVISTIC EXPLOSION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Very-long-baseline interferometry; Equipartition theorem; Astrophysical jet; Astronomy; Observatory; Active galactic nucleus; Galaxy; Magnetic field","score_opus":0.018786076511207953,"score_gpt":0.241041681421603,"score_spread":0.22225560491039506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2058998647","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953199,0.00018367937,0.00053455355,0.000026704083,0.0000091288075,0.000012645698,0.00043696217,0.00006163788,0.0034147978],"genre_scores_gemma":[0.99545825,0.00017591863,0.002211781,0.00008342887,0.000022757647,0.0000080617365,0.0014726613,0.000012478739,0.0005546366],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999404,0.0000036068134,0.0000035151163,0.000019663868,0.000015029164,0.000017863122],"domain_scores_gemma":[0.999778,0.000019920373,0.00008743108,0.0000394674,0.0000203128,0.000054955563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013848669,0.00026551037,0.00020426838,0.0005629843,0.00024290723,0.0003696074,0.0002910938,0.00034417398,0.0006255318],"category_scores_gemma":[0.00017639816,0.000112932656,0.0002275149,0.00047538412,0.0002283564,0.00016486332,0.00028560124,0.00030650393,0.0003294836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039962897,0.00018712977,0.8899298,0.00011399797,0.00012449242,0.0038951724,0.0002636905,0.0012009692,0.07817826,0.0015792487,0.0022767808,0.02185082],"study_design_scores_gemma":[0.000010161115,0.0002761644,0.98713,0.000012683988,0.000029042852,0.0058118566,0.000111375324,0.0010076275,0.0025584856,0.00027852875,0.0027653603,0.000008751187],"about_ca_topic_score_codex":0.0012635671,"about_ca_topic_score_gemma":0.0050205495,"teacher_disagreement_score":0.0012635671,"about_ca_system_score_codex":0.00014304325,"about_ca_system_score_gemma":0.00010816574,"threshold_uncertainty_score":0.0025123954},"labels":[],"label_agreement":null},{"id":"W2059001712","doi":"10.1088/0004-637x/702/2/1230","title":"A ROTATION MEASURE IMAGE OF THE SKY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":422,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Sky; Halo; Galactic plane; Galactic halo; Magnetic field; Scale height; Field (mathematics); Declination; Galaxy","score_opus":0.005914726486006074,"score_gpt":0.2118028540883053,"score_spread":0.20588812760229921,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059001712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5184961,0.0010995991,0.14340697,0.00088549365,0.000485541,0.00051365973,0.1383589,0.017236482,0.17951725],"genre_scores_gemma":[0.73064,0.00052032573,0.14344397,0.0002616472,0.0002649039,0.00021560353,0.093895055,0.0018880883,0.028870393],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982774,0.000013561993,0.00000769866,0.000048869177,0.00007226034,0.000029807221],"domain_scores_gemma":[0.99970007,0.000017414046,0.000031430653,0.000077978424,0.00012863347,0.000044513552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015543924,0.00024472838,0.00021325059,0.0017949697,0.00020417685,0.00060085696,0.00023326883,0.00019945185,0.016322417],"category_scores_gemma":[0.00041841876,0.0001688658,0.0003131044,0.0015256264,0.000104980536,0.00034351213,0.00040623025,0.00035640973,0.005079615],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006846933,0.00018703804,0.06629627,0.0004166497,0.00020404928,0.0003767054,0.0005689341,0.0048904154,0.32245818,0.006418911,0.09267569,0.5048225],"study_design_scores_gemma":[0.00009885904,0.00020746076,0.6753082,0.00007216533,0.00010556138,0.0010272536,0.00026094247,0.022212185,0.033137288,0.0018641516,0.26564616,0.00005977634],"about_ca_topic_score_codex":0.007378485,"about_ca_topic_score_gemma":0.010368944,"teacher_disagreement_score":0.016322417,"about_ca_system_score_codex":0.00036078345,"about_ca_system_score_gemma":0.00040935492,"threshold_uncertainty_score":0.054603875},"labels":[],"label_agreement":null},{"id":"W2059069810","doi":"10.1088/0004-637x/793/1/11","title":"IMAGING THE ENVIRONMENT OF A<i>z</i>= 6.3 SUBMILLIMETER GALAXY WITH SCUBA-2","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Dalhousie University; University of British Columbia","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Centre National de la Recherche Scientifique; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Centre National d’Etudes Spatiales; Danmarks Grundforskningsfond; Cardiff University; University of Sussex; Leverhulme Trust; Science and Technology Facilities Council; National Research Foundation; UK Space Agency; Imperial College London; University of Lethbridge; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Galaxy; Galactic astronomy; Radio astronomy; Submillimeter Array; Extragalactic astronomy; Galaxy cluster; Submillimeter wave; Radio galaxy","score_opus":0.004032278710129226,"score_gpt":0.17473342919654442,"score_spread":0.17070115048641518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059069810","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911301,0.000067265355,0.0025514644,0.00015964014,0.000011805432,0.000012258743,0.00048704862,0.00029880847,0.005281642],"genre_scores_gemma":[0.991667,0.000030311347,0.007083903,0.00011050062,0.000009793505,0.000007640236,0.00057546207,0.000046249315,0.00046915963],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994123,0.0000056558147,0.0000013874084,0.000013393169,0.000016057431,0.000022151014],"domain_scores_gemma":[0.99983406,0.000020670592,0.000029855175,0.000027723743,0.000015021735,0.000072686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023861813,0.00014052754,0.00012971566,0.0003499008,0.00029169442,0.00037589646,0.00045861574,0.0002777451,0.0011506282],"category_scores_gemma":[0.00024314102,0.0001310023,0.00032284035,0.0002891413,0.00018556233,0.0002535008,0.0003949094,0.00037651815,0.00026547138],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059222017,0.0003769079,0.7131448,0.00011135226,0.00027688037,0.001759758,0.0012260004,0.032155395,0.19702642,0.0066382624,0.010179917,0.03651217],"study_design_scores_gemma":[0.00006629345,0.00024053316,0.8524874,0.000029676894,0.00008884319,0.0010728269,0.00040384848,0.1158918,0.019098004,0.0023126863,0.008247723,0.000060362483],"about_ca_topic_score_codex":0.0054509654,"about_ca_topic_score_gemma":0.011261183,"teacher_disagreement_score":0.0054509654,"about_ca_system_score_codex":0.0004054265,"about_ca_system_score_gemma":0.00019536467,"threshold_uncertainty_score":0.010838449},"labels":[],"label_agreement":null},{"id":"W2059091879","doi":"10.1086/505169","title":"A Study of Compact Object Mergers as Short Gamma‐Ray Burst Progenitors","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":297,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Gamma-ray burst; Neutron star; Compact star; Afterglow; Galaxy; Host (biology); Population; Stars","score_opus":0.01234554143065543,"score_gpt":0.2524962205734153,"score_spread":0.2401506791427599,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059091879","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9630766,0.0014222445,0.029566204,0.0001718796,0.000010178494,0.000019934187,0.0000489996,0.00003967072,0.0056442562],"genre_scores_gemma":[0.99315673,0.00071402773,0.004702312,0.000016001959,0.000022607996,0.000015817792,0.00009622643,0.000012556069,0.0012637748],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998847,0.000032535696,0.0000053911203,0.000026381198,0.000026485055,0.000024484256],"domain_scores_gemma":[0.9990513,0.00043720732,0.00022164176,0.0000837004,0.00007336632,0.00013276919],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038842493,0.0003705116,0.00031069727,0.00074550166,0.0006477525,0.0011659169,0.0006681615,0.0004835602,0.0017742359],"category_scores_gemma":[0.0020780792,0.00027089854,0.0004196567,0.0007374321,0.00060955936,0.0013033163,0.00068730797,0.0003246345,0.00027548417],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003548423,0.00024407591,0.20603839,0.00029367956,0.00012524497,0.004178615,0.0015881846,0.2723095,0.02597646,0.4110534,0.001634728,0.076202996],"study_design_scores_gemma":[0.000054594348,0.00041790612,0.039493244,0.00006226831,0.00009310587,0.0045631644,0.00059646735,0.84656805,0.005363304,0.093959235,0.008790444,0.00003826793],"about_ca_topic_score_codex":0.0013878378,"about_ca_topic_score_gemma":0.00070187735,"teacher_disagreement_score":0.0017742359,"about_ca_system_score_codex":0.0004981623,"about_ca_system_score_gemma":0.0004087215,"threshold_uncertainty_score":0.005935371},"labels":[],"label_agreement":null},{"id":"W2059215206","doi":"10.1086/587051","title":"Variations of the Mid‐IR Aromatic Features inside and among Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":298,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Astrophysics; Physics; Galaxy; Spiral galaxy; Ionization; Extinction (optical mineralogy); Spectral line; Irregular galaxy; Bar (unit); Star formation; Astronomy; Lenticular galaxy; Ion","score_opus":0.008567452769901583,"score_gpt":0.21110369228971007,"score_spread":0.20253623951980848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059215206","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877566,0.00016645265,0.00028041872,0.000003805527,6.4361365e-7,0.0000020518355,0.00022503824,0.000017363664,0.0005285871],"genre_scores_gemma":[0.99903893,0.00007949429,0.00029615418,0.0000039593806,0.000004327067,0.0000032296052,0.0003852521,0.0000070677897,0.00018162356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999744,0.000029747474,0.0000146347875,0.000120969235,0.000044055414,0.00004650074],"domain_scores_gemma":[0.9986123,0.0002950843,0.0005250599,0.00022907427,0.00018361017,0.00015491489],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023242386,0.00021022338,0.0002642333,0.0022890978,0.00036376552,0.00056095026,0.0002829657,0.00023074156,0.00088074687],"category_scores_gemma":[0.0007642698,0.00017709097,0.00032402968,0.0013062995,0.0003604828,0.00035183333,0.0004548784,0.00015764177,0.00036116646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000066523935,0.000023233519,0.9558651,0.00003164816,0.000089616915,0.00007167732,0.00042948316,0.00028083715,0.032861456,0.00011635465,0.00005529073,0.010108861],"study_design_scores_gemma":[3.6663482e-7,0.000018827477,0.9986578,0.0000014768904,0.000013861345,0.00008900424,0.00005080836,0.00008789319,0.00090336223,0.000017496333,0.00015721611,0.0000017477663],"about_ca_topic_score_codex":0.001165117,"about_ca_topic_score_gemma":0.0017407574,"teacher_disagreement_score":0.0022890978,"about_ca_system_score_codex":0.00017891738,"about_ca_system_score_gemma":0.00006212552,"threshold_uncertainty_score":0.0029463768},"labels":[],"label_agreement":null},{"id":"W2059327536","doi":"10.1086/431281","title":"An Upper Limit on the Expansion Velocity of Gamma-Ray Burst Candidate SN 2001em","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Angular diameter; RADIUS; Supernova; Angular resolution (graph drawing); Line-of-sight; Very-long-baseline interferometry; Jet (fluid); Isotropy","score_opus":0.012117711337516712,"score_gpt":0.23819329726633828,"score_spread":0.22607558592882157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059327536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879423,0.00086289,0.0024269964,0.00007072782,0.000021651971,0.000012120858,0.00054590125,0.00007845906,0.008039009],"genre_scores_gemma":[0.99309456,0.00034328687,0.0021731146,0.00007583128,0.000028039898,0.000021433732,0.0030451072,0.000025480656,0.0011931154],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998919,0.000018222201,0.00000936387,0.000031943284,0.00002109875,0.000027436146],"domain_scores_gemma":[0.9994524,0.00016437215,0.00014297281,0.000058582547,0.00010680122,0.00007487364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005805428,0.00023484431,0.00017738283,0.0006261369,0.00028796057,0.0005377229,0.00022190502,0.00036556373,0.0020857102],"category_scores_gemma":[0.0009688414,0.000111752146,0.0001567858,0.00027300962,0.00016741392,0.0003361659,0.00041246752,0.0003512527,0.00065668754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000689188,0.00013055337,0.81500876,0.00014237894,0.000061341976,0.000848451,0.0004768449,0.0009530874,0.14270802,0.0032465057,0.0015328374,0.03420203],"study_design_scores_gemma":[0.000010495265,0.00013949901,0.9728856,0.000031891755,0.000017861494,0.001545272,0.00010929165,0.0013681215,0.012682117,0.00055514096,0.010641822,0.00001293757],"about_ca_topic_score_codex":0.0006924823,"about_ca_topic_score_gemma":0.00094958936,"teacher_disagreement_score":0.0020857102,"about_ca_system_score_codex":0.00018097287,"about_ca_system_score_gemma":0.000078993355,"threshold_uncertainty_score":0.006977439},"labels":[],"label_agreement":null},{"id":"W2059350630","doi":"10.1088/0004-637x/758/1/7","title":"SIZE OF THE VELA PULSAR'S EMISSION REGION AT 18 cm WAVELENGTH","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Vela; Physics; Pulsar; Amplitude; Astrophysics; Wavelength; Pulse (music); Visibility; Phase (matter); Scintillation; Optics; Detector","score_opus":0.018177198424739263,"score_gpt":0.30679166824440873,"score_spread":0.2886144698196695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059350630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99295133,0.00020494116,0.0018138019,0.000048261863,0.000009509907,0.000005224434,0.0011139361,0.0001367724,0.0037161543],"genre_scores_gemma":[0.9972198,0.000057142268,0.0012835767,0.000016823331,0.00001633719,0.000009667812,0.00087485794,0.000031726093,0.0004901498],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995375,0.0000040850364,0.0000017894827,0.000018801116,0.000011341612,0.0000103036555],"domain_scores_gemma":[0.99975175,0.00008169529,0.00007181189,0.000021519603,0.000029025063,0.00004412202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010393952,0.00007415809,0.000081043494,0.00053331244,0.00021103794,0.00021072589,0.00028189778,0.00010926513,0.0015419488],"category_scores_gemma":[0.0003176965,0.00009017104,0.00010111702,0.00029108796,0.00018677898,0.00018821958,0.00023851897,0.0002204083,0.00029080696],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000684435,0.000090075795,0.4773154,0.0001253737,0.00009251411,0.00042106444,0.0007109132,0.002277951,0.4414311,0.0018076901,0.0025789952,0.07246452],"study_design_scores_gemma":[0.000005261879,0.00004731732,0.9856494,0.0000059067647,0.000012844278,0.00026992048,0.000038147362,0.001304468,0.010975115,0.0001342896,0.0015507126,0.000006518842],"about_ca_topic_score_codex":0.0005785837,"about_ca_topic_score_gemma":0.00071576255,"teacher_disagreement_score":0.0015419488,"about_ca_system_score_codex":0.00015895479,"about_ca_system_score_gemma":0.00005653043,"threshold_uncertainty_score":0.005158305},"labels":[],"label_agreement":null},{"id":"W2059351082","doi":"10.1086/521542","title":"An Extremely Bright Echo Associated with SN 2002hh","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Supernova; Photometry (optics); Physics; Brightness; Extinction (optical mineralogy); Spectral line; Light curve; Echo (communications protocol); Pair-instability supernova; Astronomy; Optics; Stars; Ejecta","score_opus":0.01063854793476618,"score_gpt":0.2315606317058947,"score_spread":0.2209220837711285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059351082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99722666,0.00009325566,0.0006682811,0.000029466151,0.000015810558,0.000005696715,0.00024909593,0.0000739483,0.0016378369],"genre_scores_gemma":[0.9974739,0.00004031592,0.0009994077,0.00003175061,0.000029745044,0.0000022990002,0.00072661764,0.0000124831795,0.00068342587],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993515,0.000002940522,0.0000034451543,0.000017847531,0.000020991742,0.000019655852],"domain_scores_gemma":[0.999747,0.000017659002,0.00008201833,0.00003009931,0.000034876208,0.000088296445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009423491,0.00023803391,0.0001447631,0.00066102773,0.00032750843,0.00039403976,0.00017808645,0.00026498715,0.0011431114],"category_scores_gemma":[0.00014557647,0.00010230775,0.00013011815,0.00040496723,0.00013797186,0.0001690809,0.00040139304,0.00020520441,0.00028087138],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003334184,0.00015716246,0.8165459,0.00007183396,0.00007327305,0.005886976,0.00046593486,0.00027510288,0.14096978,0.000526533,0.0020587146,0.032635257],"study_design_scores_gemma":[0.000006097777,0.00010803024,0.98539746,0.00000463309,0.000019860869,0.0044077975,0.00014171883,0.00063929724,0.0064908084,0.00010534712,0.0026683812,0.000010553631],"about_ca_topic_score_codex":0.002575188,"about_ca_topic_score_gemma":0.009276051,"teacher_disagreement_score":0.002575188,"about_ca_system_score_codex":0.00011894054,"about_ca_system_score_gemma":0.00009156976,"threshold_uncertainty_score":0.005120337},"labels":[],"label_agreement":null},{"id":"W2059438168","doi":"10.1088/0004-637x/772/1/51","title":"OPTICAL PHASE CURVES OF<i>KEPLER</i>EXOPLANETS","year":2013,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":176,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planet; Physics; Light curve; Exoplanet; Astrophysics; Astronomy; Spitzer Space Telescope; Kepler; Radial velocity; Stars","score_opus":0.013575637110696074,"score_gpt":0.24523246272260524,"score_spread":0.23165682561190917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059438168","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981567,0.00007837199,0.00035462045,0.0000070169194,0.0000011948613,0.000003740705,0.00035521344,0.000040281044,0.0010027123],"genre_scores_gemma":[0.99779046,0.000052044696,0.00072787626,0.0000065709737,0.000003122232,0.0000050594467,0.0010046024,0.000024352252,0.00038600134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999137,0.0000071200493,0.000008102494,0.000033155717,0.000015110263,0.000022779486],"domain_scores_gemma":[0.99956745,0.0000683493,0.00018354793,0.000047642025,0.00007293641,0.00006016144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014192075,0.00019819914,0.00022080966,0.0010460134,0.00031229173,0.00039238707,0.00016296374,0.00012783693,0.0012504857],"category_scores_gemma":[0.0006390498,0.0001517901,0.0002153256,0.00089868915,0.00012826991,0.00028462402,0.00029094535,0.00013706261,0.0003760807],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041887604,0.000055289976,0.9063455,0.00007945653,0.0000786275,0.00016412402,0.00040677996,0.0028585345,0.057500377,0.0002942979,0.00051920884,0.031278934],"study_design_scores_gemma":[0.000007958667,0.00010993834,0.9901216,0.000004671223,0.000026851798,0.0002904176,0.00009607831,0.0019604366,0.0053482982,0.00010407502,0.0019219319,0.000007863666],"about_ca_topic_score_codex":0.0019479314,"about_ca_topic_score_gemma":0.002976061,"teacher_disagreement_score":0.0019479314,"about_ca_system_score_codex":0.0003176638,"about_ca_system_score_gemma":0.00009564703,"threshold_uncertainty_score":0.004183233},"labels":[],"label_agreement":null},{"id":"W2059515425","doi":"10.1086/386302","title":"GSH 23.0−0.7+117: A Neutral Hydrogen Shell in the Inner Galaxy","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Calgary","funders":"","keywords":"Physics; Astrophysics; Galaxy; Shell (structure); RADIUS; Galactic plane","score_opus":0.010008727633540618,"score_gpt":0.2311204575571357,"score_spread":0.22111172992359507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059515425","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99635065,0.000042255255,0.0001067689,0.000018065844,0.0000033455758,0.0000076284464,0.00048550277,0.000050468607,0.0029352226],"genre_scores_gemma":[0.9976921,0.000021012334,0.00029462017,0.000017573062,0.0000036441013,0.000003874907,0.0008593054,0.000016537517,0.0010913586],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994457,0.0000028834547,0.0000017420422,0.000012666588,0.0000119385095,0.000026186102],"domain_scores_gemma":[0.9998708,0.0000019373904,0.000021834298,0.0000081965645,0.000010138128,0.00008708958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005906913,0.00018731083,0.00021139056,0.0003531104,0.00034970974,0.00049562054,0.0002134823,0.00021772308,0.0031310427],"category_scores_gemma":[0.000105669016,0.00010625233,0.00019516023,0.00032642708,0.00019522948,0.00013309675,0.00046598862,0.00015907822,0.0013277835],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046400825,0.0001916457,0.8710601,0.00006482681,0.00009774574,0.0025319718,0.000837967,0.000594863,0.09839442,0.0019536316,0.0032782746,0.0205306],"study_design_scores_gemma":[0.000014735051,0.00015154104,0.98756474,0.0000067906976,0.000022443857,0.0012016471,0.00027587533,0.0004520363,0.0032681026,0.00019514322,0.006838299,0.000008681543],"about_ca_topic_score_codex":0.013395313,"about_ca_topic_score_gemma":0.016887674,"teacher_disagreement_score":0.013395313,"about_ca_system_score_codex":0.000507393,"about_ca_system_score_gemma":0.0002111885,"threshold_uncertainty_score":0.026634693},"labels":[],"label_agreement":null},{"id":"W2059519221","doi":"10.1086/381387","title":"Globular Cluster Archaeology: Hydrogen‐burning Nucleosynthesis and Extra Mixing in Extinct Stars","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Globular cluster; Asymptotic giant branch; Nucleosynthesis; Astrophysics; Stars; Red giant; Red-giant branch; Astronomy; Horizontal branch; Star cluster; Stellar nucleosynthesis; Stellar evolution; Giant star","score_opus":0.009133668401139345,"score_gpt":0.21429423963544186,"score_spread":0.2051605712343025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059519221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99921024,0.000028685976,0.0003242681,0.000013169241,0.0000010339561,0.0000011563326,0.000069109316,0.0000082920205,0.0003440202],"genre_scores_gemma":[0.9991872,0.00001993554,0.00041897624,0.0000036093286,0.0000017779864,0.0000015013826,0.00018448928,0.0000051875236,0.00017740214],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999459,0.000009772902,0.0000025668962,0.000018278968,0.000009120803,0.000014248878],"domain_scores_gemma":[0.9996375,0.00011859987,0.00006956221,0.000056789635,0.00003838806,0.000079107085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028428558,0.00021148511,0.00018646724,0.00040987134,0.00040460835,0.0004483968,0.00037789793,0.00045966663,0.0009661926],"category_scores_gemma":[0.0016376559,0.00018775804,0.00023300853,0.00060413213,0.00048086778,0.00033861736,0.00040505722,0.00019464121,0.00013863441],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026324976,0.00003329403,0.6737148,0.000027005379,0.000081096645,0.00028324724,0.00022420862,0.31416523,0.0032989993,0.0032824103,0.00024597955,0.004380393],"study_design_scores_gemma":[0.000045023604,0.000048273207,0.42749447,0.00000876129,0.0000455024,0.00031377168,0.00022609698,0.56519246,0.0026778707,0.0030948215,0.0008337923,0.000019203531],"about_ca_topic_score_codex":0.0310646,"about_ca_topic_score_gemma":0.027239403,"teacher_disagreement_score":0.0310646,"about_ca_system_score_codex":0.00068891066,"about_ca_system_score_gemma":0.00047200892,"threshold_uncertainty_score":0.061767578},"labels":[],"label_agreement":null},{"id":"W2059554882","doi":"10.1086/426684","title":"Evaluating the Magnetic Field Strength in Molecular Clouds","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Molecular cloud; Field strength; Magnetic field; Orientation (vector space); Field (mathematics); Extension (predicate logic)","score_opus":0.01507153883825842,"score_gpt":0.28989997937733125,"score_spread":0.27482844053907285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059554882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6883662,0.0018446859,0.29988742,0.00044662328,0.00012370151,0.000085637745,0.00030789422,0.0005942839,0.008343568],"genre_scores_gemma":[0.9409027,0.0005250256,0.057074316,0.00003493912,0.00006470997,0.000026703228,0.00010796073,0.00006815891,0.0011954599],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998553,0.000029586343,0.0000059496633,0.000016439319,0.000062209714,0.00003048772],"domain_scores_gemma":[0.99939716,0.00024707208,0.00010536777,0.00004037012,0.00013235389,0.00007766724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005568362,0.00040195955,0.0005101842,0.0008863123,0.00058859336,0.0007770705,0.0010162668,0.0004803341,0.0010454042],"category_scores_gemma":[0.0028769332,0.0002077246,0.0003208955,0.00067868124,0.00033586606,0.0008518164,0.0008489839,0.0004688187,0.0002555543],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041948608,0.00013732511,0.058127306,0.0003754326,0.00016348652,0.0008797407,0.00027880233,0.6216794,0.10461626,0.042128034,0.0014043248,0.16979033],"study_design_scores_gemma":[0.00004873262,0.000052229894,0.011791614,0.000027238804,0.000024229883,0.00017780185,0.0000641598,0.9538793,0.0234526,0.008816557,0.0016065479,0.000058957365],"about_ca_topic_score_codex":0.010367443,"about_ca_topic_score_gemma":0.008300429,"teacher_disagreement_score":0.010367443,"about_ca_system_score_codex":0.0006980497,"about_ca_system_score_gemma":0.0008240686,"threshold_uncertainty_score":0.020614207},"labels":[],"label_agreement":null},{"id":"W2059563181","doi":"10.1086/323568","title":"Measurement of the Bias Parameter from Weak Lensing","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmology; Galaxy; Weak gravitational lensing; Correlation function (quantum field theory); Scale (ratio); Galaxy cluster; Dark matter; Sample (material); Measure (data warehouse)","score_opus":0.026843654908795922,"score_gpt":0.21778817923057378,"score_spread":0.19094452432177786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059563181","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99512094,0.00013745429,0.003278407,0.000021582242,0.000003751884,0.0000050467575,0.00027219605,0.000057506724,0.0011029835],"genre_scores_gemma":[0.9982626,0.000050629296,0.0012405172,0.000009488906,0.0000075665143,0.0000028925845,0.00027705272,0.00000958729,0.00013972065],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995303,0.00008641752,0.000030789382,0.00012700567,0.00014728561,0.00007829541],"domain_scores_gemma":[0.99542147,0.0016881638,0.0014186315,0.0005623189,0.00057410344,0.00033535052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087918184,0.0002664314,0.00023924322,0.0011107012,0.00013785652,0.00042465093,0.0002882201,0.00019567656,0.0012134059],"category_scores_gemma":[0.0055895406,0.00014463726,0.00013110453,0.0007493264,0.0003301165,0.00049650733,0.00063120225,0.00035888783,0.00031398205],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015337848,0.000025887433,0.9148323,0.00005639843,0.000119324795,0.00007345431,0.00010692992,0.0025621902,0.06551819,0.0011490153,0.00018939807,0.01521331],"study_design_scores_gemma":[0.0000065388645,0.0001493109,0.95888555,0.000010797773,0.000043334137,0.0002498218,0.0000479324,0.009464248,0.029236246,0.0011557848,0.0007192079,0.000031337022],"about_ca_topic_score_codex":0.0017686161,"about_ca_topic_score_gemma":0.0018981219,"teacher_disagreement_score":0.0017686161,"about_ca_system_score_codex":0.0003172655,"about_ca_system_score_gemma":0.0001432462,"threshold_uncertainty_score":0.004649639},"labels":[],"label_agreement":null},{"id":"W2059577883","doi":"10.1086/429667","title":"Discovery of Photospheric Germanium in Hot DA White Dwarfs","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; White dwarf; Photosphere; Germanium; Stars; Line (geometry); Spectral line; Astronomy; Abundance (ecology); Stellar classification; Main sequence; Silicon","score_opus":0.008797165946831945,"score_gpt":0.22035206923446515,"score_spread":0.2115549032876332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059577883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995129,0.000070200804,0.00010394239,0.000006305648,7.550043e-7,8.885959e-7,0.000041856816,0.00000503396,0.0002581402],"genre_scores_gemma":[0.9995807,0.00003755902,0.0001384569,0.0000068693903,0.0000014034517,9.0097166e-7,0.00007010112,0.0000027300218,0.00016128235],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996185,0.000002722928,0.0000017127429,0.000015344123,0.0000074794275,0.000010922168],"domain_scores_gemma":[0.9999409,0.000006740353,0.000022704933,0.000006969505,0.0000075533453,0.000015275325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000057014975,0.00016558361,0.00013113479,0.00046662765,0.00030754448,0.00036818825,0.00012917293,0.00024486982,0.00046229258],"category_scores_gemma":[0.00010910927,0.000116863615,0.00006326774,0.0001807566,0.00026795297,0.00015484012,0.00030308435,0.00009762441,0.00011484846],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002612555,0.000019796606,0.20588115,0.00004181272,0.000046338817,0.00051296485,0.00062122964,0.000078152436,0.786172,0.0002646248,0.000080712125,0.0060200505],"study_design_scores_gemma":[0.000013865213,0.0001514326,0.87460047,0.000007788724,0.000046204554,0.0016944184,0.00054974493,0.0004756605,0.119639434,0.00031373432,0.0024965717,0.000010565374],"about_ca_topic_score_codex":0.0011691109,"about_ca_topic_score_gemma":0.0021762415,"teacher_disagreement_score":0.0011691109,"about_ca_system_score_codex":0.00011864668,"about_ca_system_score_gemma":0.00004676582,"threshold_uncertainty_score":0.0023245811},"labels":[],"label_agreement":null},{"id":"W2059685496","doi":"10.1088/0004-637x/782/2/113","title":"SHEDDING LIGHT ON THE ECCENTRICITY VALLEY: GAP HEATING AND ECCENTRICITY EXCITATION OF GIANT PLANETS IN PROTOPLANETARY DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Planet; Astrophysics; Exoplanet; Tidal heating; Protoplanetary disk; Planetary system; Sublimation (psychology); Barotropic fluid; Eccentricity (behavior); Giant planet; Astronomy; Mechanics","score_opus":0.011946440927320869,"score_gpt":0.23246037124736663,"score_spread":0.22051393032004576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059685496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99909747,0.0000719878,0.00020066035,0.000028765166,0.0000015145828,6.3766345e-7,0.000012660771,0.000005887991,0.00058040215],"genre_scores_gemma":[0.99986506,0.000011706132,0.000043981614,0.000003755063,0.0000016470824,2.2838086e-7,0.0000064888723,0.0000018875269,0.00006533379],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999702,0.0000029405135,0.0000010744699,0.000008268483,0.00000640907,0.00001112352],"domain_scores_gemma":[0.99987316,0.000031961517,0.000041327843,0.00001352577,0.000008672705,0.000031292613],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005190834,0.00009689894,0.00013740468,0.00020072839,0.00031288865,0.0003502626,0.00018073937,0.00024325629,0.00086731015],"category_scores_gemma":[0.0003598953,0.00009901762,0.000109639506,0.00011599928,0.0003654771,0.00023135354,0.0005277729,0.00028937985,0.000108735774],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082029955,0.00017324601,0.53532076,0.00014300246,0.00006401886,0.0034117517,0.0032957196,0.012777246,0.40791756,0.0046015796,0.0013691478,0.030105637],"study_design_scores_gemma":[0.00002142656,0.00012775771,0.94871885,0.0000134952215,0.000017592663,0.001643481,0.00095389027,0.02601306,0.015943844,0.005360923,0.001164089,0.00002163819],"about_ca_topic_score_codex":0.00082548877,"about_ca_topic_score_gemma":0.0011836365,"teacher_disagreement_score":0.00086731015,"about_ca_system_score_codex":0.00018584669,"about_ca_system_score_gemma":0.000056509085,"threshold_uncertainty_score":0.002901435},"labels":[],"label_agreement":null},{"id":"W2059795572","doi":"10.1086/339498","title":"Understanding the Nature of Optically Faint Radio Sources and Their Connection to the Submillimeter Population","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Redshift; Astrophysics; Galaxy; Luminosity; Population; Astronomy; Sample (material); Radio galaxy","score_opus":0.017443794285963307,"score_gpt":0.20427828023561576,"score_spread":0.18683448594965246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059795572","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973437,0.00024142447,0.0011998081,0.00010796367,0.0000013396427,0.0000060965835,0.00012450611,0.000008545302,0.00096665206],"genre_scores_gemma":[0.99879944,0.00017282474,0.0004889512,0.000029521014,0.000008197096,0.000006484436,0.00020896067,0.000003956416,0.00028160276],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999826,0.00003801692,0.0000066003545,0.00005304528,0.000024739118,0.000051559473],"domain_scores_gemma":[0.9981902,0.0006893961,0.0007022002,0.00020210313,0.000098908924,0.000117228396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051564816,0.00024536363,0.00024456182,0.0011308603,0.0002931715,0.0010271721,0.00044217336,0.0005597264,0.0023889178],"category_scores_gemma":[0.003544113,0.0002343864,0.00017649152,0.0008937586,0.00036020455,0.0012797609,0.00058837514,0.00039511558,0.00044278582],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000053060463,0.000030144554,0.979996,0.000016510088,0.00001726254,0.000077576115,0.00043646534,0.0013370602,0.003268613,0.002041512,0.00012652854,0.012599283],"study_design_scores_gemma":[0.0000027952728,0.000024765133,0.99210405,0.000005612204,0.000013056731,0.00017178955,0.0003357984,0.0044017816,0.00029015858,0.0021761719,0.00046901806,0.0000050636804],"about_ca_topic_score_codex":0.004168425,"about_ca_topic_score_gemma":0.00533129,"teacher_disagreement_score":0.004168425,"about_ca_system_score_codex":0.0002996246,"about_ca_system_score_gemma":0.00018712481,"threshold_uncertainty_score":0.008288324},"labels":[],"label_agreement":null},{"id":"W2059809812","doi":"10.1086/338754","title":"On Quasar Distances and Lifetimes in a Local Model","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"QSOS; Quasar; Redshift; Galaxy; Luminosity; Cosmology; Hubble's law","score_opus":0.008324238947142501,"score_gpt":0.20300523456786604,"score_spread":0.19468099562072355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059809812","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9414982,0.0020597682,0.024549888,0.0012389971,0.000024440486,0.000022460385,0.00049240905,0.00011988865,0.029993854],"genre_scores_gemma":[0.99575305,0.00050077215,0.000709345,0.000045687295,0.000023519508,0.000012700934,0.00013284094,0.00002960325,0.0027925048],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997247,0.000069079506,0.000011250805,0.000090267975,0.00003161466,0.00007321231],"domain_scores_gemma":[0.99319696,0.0037901497,0.0014648493,0.00060260046,0.00041528768,0.00053010194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017914352,0.00033184222,0.00032597178,0.00092223025,0.00069358596,0.0016222309,0.0008342623,0.00074229384,0.004700489],"category_scores_gemma":[0.011423223,0.00018767892,0.0003413492,0.00061283255,0.0011492354,0.0033831145,0.0015643433,0.00086118036,0.00078227575],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027982483,0.00007935602,0.11917255,0.00012483145,0.00010590984,0.0008196646,0.0024790955,0.27946365,0.0011936107,0.5553507,0.0023832454,0.038547505],"study_design_scores_gemma":[0.000082439845,0.00024261551,0.06607939,0.00013995646,0.00021875811,0.0017542868,0.0014778628,0.5169425,0.00063647464,0.3992176,0.013101302,0.00010687368],"about_ca_topic_score_codex":0.005561087,"about_ca_topic_score_gemma":0.0043349275,"teacher_disagreement_score":0.005561087,"about_ca_system_score_codex":0.0016753754,"about_ca_system_score_gemma":0.00034545848,"threshold_uncertainty_score":0.015724659},"labels":[],"label_agreement":null},{"id":"W2059925651","doi":"10.1088/0004-637x/785/2/119","title":"GRAVITATIONAL WAVES FROM KNOWN PULSARS: RESULTS FROM THE INITIAL DETECTOR ERA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":182,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Istituto Nazionale di Fisica Nucleare; Ministero dello Sviluppo Economico; National Research Foundation of Korea; Ministerio de Economía y Competitividad; Centre National de la Recherche Scientifique; Industry Canada; Govern de les Illes Balears; Fundacja na rzecz Nauki Polskiej; Scottish Funding Council; Institut des Origines de Lyon; Scottish Universities Physics Alliance; Hungarian Scientific Research Fund; Leverhulme Trust; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Council of Scientific and Industrial Research, India; Science and Technology Facilities Council; National Research Foundation; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Pulsar; LIGO; Physics; Gravitational wave; Gravitational-wave observatory; Millisecond pulsar; Astronomy; Vela; Astrophysics; Gravitational-wave astronomy; Neutron star; Observatory; Detector; Interferometry; Amplitude; Optics","score_opus":0.017915034869823588,"score_gpt":0.3131245012907593,"score_spread":0.2952094664209357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059925651","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97346175,0.0073356843,0.0067545697,0.00017176203,0.00002872995,0.00004337398,0.0056825066,0.00026657525,0.0062549226],"genre_scores_gemma":[0.96402955,0.0035270364,0.012299618,0.00013573513,0.00008991725,0.00005069532,0.01779878,0.00011830845,0.0019504392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985701,0.0002364042,0.00011411065,0.00032999273,0.0005557584,0.0001935398],"domain_scores_gemma":[0.9953302,0.0024698675,0.00064973807,0.0006053649,0.00057490554,0.00036996376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021056812,0.00055356533,0.00062942825,0.0030067374,0.00066761853,0.0013314266,0.0005389626,0.0004909451,0.001403473],"category_scores_gemma":[0.0042166067,0.0003112748,0.0006561255,0.0026857033,0.00073025696,0.0010536435,0.0020622283,0.00058789895,0.0008365051],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016136208,0.00038385577,0.7889818,0.000713665,0.00068364496,0.00042714467,0.0010593894,0.0021336307,0.048049334,0.0018712347,0.002627055,0.1514557],"study_design_scores_gemma":[0.00010023352,0.0006626279,0.8983951,0.000085117725,0.00055068015,0.0013249241,0.00035123705,0.0022303013,0.06246387,0.0013667248,0.032368887,0.000100262776],"about_ca_topic_score_codex":0.0010125595,"about_ca_topic_score_gemma":0.0018624823,"teacher_disagreement_score":0.0030067374,"about_ca_system_score_codex":0.0004980011,"about_ca_system_score_gemma":0.0002503934,"threshold_uncertainty_score":0.011136055},"labels":[],"label_agreement":null},{"id":"W2059952881","doi":"10.1088/0004-637x/721/2/1593","title":"ON THE STABILITY OF DUST-LADEN PROTOPLANETARY VORTICES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planetesimal; Physics; Instability; Vortex; Protoplanetary disk; Astrophysics; Planet; Mechanics","score_opus":0.012555820798222152,"score_gpt":0.23375989677304443,"score_spread":0.22120407597482228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059952881","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99212,0.000751764,0.0042974013,0.00019949344,0.000019532123,0.0000064861997,0.000011071966,0.00001416642,0.002580095],"genre_scores_gemma":[0.99922645,0.0001693116,0.0002815829,0.000010426863,0.000016897648,0.00000256258,0.000007261595,0.0000031939608,0.00028227307],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993706,0.000014345737,0.0000024745818,0.000009507597,0.000015063825,0.000021508],"domain_scores_gemma":[0.99955076,0.00015862624,0.00012194467,0.000022360318,0.00008982346,0.000056493085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022422559,0.00015806532,0.0002127524,0.0005509854,0.0004892948,0.0008134464,0.00026223058,0.00023274029,0.00059151865],"category_scores_gemma":[0.0013759087,0.000116927375,0.0001252066,0.00013839825,0.0009588151,0.0005359501,0.00049107475,0.0002479257,0.00010609924],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014151701,0.0004217066,0.07783029,0.00034878118,0.00018293092,0.0020242708,0.0027678504,0.18360223,0.40612242,0.26491082,0.00324791,0.057125572],"study_design_scores_gemma":[0.00008928244,0.00026963867,0.03380305,0.000054605523,0.00002949306,0.00030943545,0.00059046736,0.88733166,0.017930895,0.057799127,0.0017386675,0.00005370627],"about_ca_topic_score_codex":0.0011223396,"about_ca_topic_score_gemma":0.0007431315,"teacher_disagreement_score":0.0011223396,"about_ca_system_score_codex":0.00039090315,"about_ca_system_score_gemma":0.00018235321,"threshold_uncertainty_score":0.0028362274},"labels":[],"label_agreement":null},{"id":"W2059967217","doi":"10.1088/0004-637x/752/1/23","title":"THE COSMOLOGICAL IMPACT OF LUMINOUS TeV BLAZARS. II. REWRITING THE THERMAL HISTORY OF THE INTERGALACTIC MEDIUM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Reionization; Blazar; Cosmic microwave background; Luminosity; Quasar; Opacity; Compton scattering; Extragalactic background light; Intergalactic travel; Fermi Gamma-ray Space Telescope","score_opus":0.011865356100142431,"score_gpt":0.23089893373221498,"score_spread":0.21903357763207254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2059967217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9625648,0.0039243167,0.0054595,0.0011642141,0.000048632923,0.000012331499,0.0005379417,0.00014644026,0.026141787],"genre_scores_gemma":[0.99598855,0.0008608963,0.0014708072,0.00010750874,0.00005424305,0.0000050569843,0.00020661009,0.000053340096,0.0012529833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998567,0.00003880465,0.0000035816586,0.000038007827,0.000026451198,0.000036467925],"domain_scores_gemma":[0.99945873,0.00008808456,0.000222356,0.00008179935,0.00002301797,0.00012608305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035832662,0.00049446133,0.00020205275,0.00079381943,0.0005254907,0.0016573644,0.0005878062,0.000493264,0.0035383399],"category_scores_gemma":[0.0014078477,0.00036128427,0.00038982098,0.00074547005,0.00088795595,0.0012915898,0.0012793648,0.0010653152,0.00034016592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044498625,0.00017403798,0.4356294,0.0005067104,0.00038794387,0.002996663,0.004584055,0.023275113,0.06917248,0.38291538,0.003970867,0.07594231],"study_design_scores_gemma":[0.00003435651,0.0001146992,0.9001086,0.00010947201,0.00014139345,0.0013571096,0.0011570601,0.01573821,0.003630384,0.062051773,0.015466492,0.00009046332],"about_ca_topic_score_codex":0.006178468,"about_ca_topic_score_gemma":0.008178544,"teacher_disagreement_score":0.006178468,"about_ca_system_score_codex":0.0011412019,"about_ca_system_score_gemma":0.00021836528,"threshold_uncertainty_score":0.012284994},"labels":[],"label_agreement":null},{"id":"W2060007384","doi":"10.1086/522791","title":"Galactic Halo Stellar Structures in the Triangulum-Andromeda Region","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Halo; Milky Way; Galactic halo; Andromeda; Stellar density; Galactic corona; Stellar structure; Young stellar object","score_opus":0.010603335265135306,"score_gpt":0.2288786450491723,"score_spread":0.218275309784037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060007384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966785,0.00056582806,0.000108093,0.000021406651,0.0000021035887,0.0000027309231,0.00013010346,0.000010814543,0.002480401],"genre_scores_gemma":[0.99909925,0.0001742561,0.00022531477,0.0000107346905,0.0000034177965,0.0000012350611,0.0002295756,0.0000042442375,0.000252007],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999145,0.000012708436,0.000004079321,0.00002281651,0.00002497248,0.000020898706],"domain_scores_gemma":[0.99974006,0.00002448368,0.000113662936,0.000023953837,0.000045293255,0.000052515195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010713543,0.00013824065,0.00014845436,0.0010939394,0.00044886293,0.0005393146,0.00017568894,0.00012725606,0.001094447],"category_scores_gemma":[0.0004453343,0.000084698055,0.00011531573,0.00082169904,0.00023504147,0.0001672362,0.00053205254,0.00011829772,0.0003022965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009699658,0.00001026461,0.95186573,0.00004227142,0.00008448315,0.0004183161,0.0013099684,0.0005373772,0.023974122,0.00079567684,0.00028496727,0.020579826],"study_design_scores_gemma":[0.000002451726,0.000013334858,0.9967914,0.000008162645,0.000012693327,0.00036931803,0.00033992005,0.000115107854,0.0005187157,0.000083445855,0.0017405141,0.0000049280948],"about_ca_topic_score_codex":0.013196598,"about_ca_topic_score_gemma":0.03433276,"teacher_disagreement_score":0.013196598,"about_ca_system_score_codex":0.00042603095,"about_ca_system_score_gemma":0.00019572675,"threshold_uncertainty_score":0.026239574},"labels":[],"label_agreement":null},{"id":"W2060014682","doi":"10.1088/0004-637x/767/1/85","title":"THE DOUBLE PULSAR: EVIDENCE FOR NEUTRON STAR FORMATION WITHOUT AN IRON CORE-COLLAPSE SUPERNOVA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Physics; Neutron star; Binary pulsar; Millisecond pulsar; Astrophysics; X-ray pulsar; Angular momentum; Supernova; X-ray binary; Orbital period; Orbital motion; Spin (aerodynamics); Classical mechanics; Stars","score_opus":0.04894854957436753,"score_gpt":0.3624231582205506,"score_spread":0.3134746086461831,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060014682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99818844,0.00030781043,0.0004061904,0.000032371307,0.000019995165,0.000006047021,0.0001315592,0.000018324217,0.00088919536],"genre_scores_gemma":[0.99911577,0.00006814839,0.00036837187,0.000029054963,0.000019754068,0.0000033838764,0.0003086822,0.000007682502,0.00007911271],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996444,0.000025490937,0.0000731732,0.00011004206,0.00009076622,0.000056067474],"domain_scores_gemma":[0.99808073,0.00032367304,0.00073184515,0.00027365447,0.0001770611,0.00041310466],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006452027,0.0003925728,0.00067592243,0.001273443,0.0005606317,0.001073681,0.00051080366,0.00068659795,0.0010243278],"category_scores_gemma":[0.002074014,0.00040181243,0.00023620877,0.0009977649,0.00089028914,0.00042406403,0.0009489273,0.00046979173,0.00047359624],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010432486,0.000109835906,0.91826683,0.00013485886,0.00015403568,0.0031098754,0.00033582936,0.00025536687,0.065141335,0.0009640245,0.00036909152,0.010115596],"study_design_scores_gemma":[0.000098529075,0.00043549878,0.97128457,0.000028766968,0.00009114318,0.016573781,0.00024513772,0.0014209826,0.0069770706,0.0008332624,0.0019916103,0.000019656994],"about_ca_topic_score_codex":0.0011640487,"about_ca_topic_score_gemma":0.0015752668,"teacher_disagreement_score":0.001273443,"about_ca_system_score_codex":0.0002601919,"about_ca_system_score_gemma":0.00027128882,"threshold_uncertainty_score":0.0034267306},"labels":[],"label_agreement":null},{"id":"W2060099785","doi":"10.1088/0004-637x/690/1/537","title":"THE HIGH-MASS END OF THE BLACK HOLE MASS FUNCTION: MASS ESTIMATES IN BRIGHTEST CLUSTER GALAXIES","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Supermassive black hole; Astronomy; Advanced Camera for Surveys; Galaxy rotation curve; Mass distribution; Stellar mass; Star cluster; Star formation; Galaxy formation and evolution","score_opus":0.006674887310522481,"score_gpt":0.19277564137570147,"score_spread":0.18610075406517898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060099785","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966826,0.0005461228,0.0004229504,0.00006568272,0.0000051861557,0.0000044642525,0.00054159464,0.000028575614,0.0017028548],"genre_scores_gemma":[0.998798,0.00011119286,0.0002553881,0.000012416111,0.000018426068,0.0000026362213,0.00037664518,0.000008394113,0.00041689945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999821,0.00003950981,0.000012184969,0.0000375721,0.000039084753,0.000050734354],"domain_scores_gemma":[0.997815,0.00057788345,0.0005805991,0.0001822026,0.00029777264,0.00054650794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009009046,0.00031321574,0.00020648802,0.0046993247,0.0003202473,0.00074554246,0.00048781527,0.0006055396,0.0035884806],"category_scores_gemma":[0.0029684291,0.00022161641,0.00018627247,0.0011366865,0.0004987997,0.0006579339,0.001005019,0.00033759105,0.0012732325],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016140468,0.000018842218,0.9875123,0.000011787257,0.000024785018,0.000063934174,0.00038137016,0.0004451815,0.0011786993,0.00024071574,0.00085172715,0.009109291],"study_design_scores_gemma":[0.0000020350094,0.000009632667,0.9991296,0.0000051506827,0.0000064287024,0.00005774152,0.00012128846,0.00025564714,0.0001891447,0.00008514499,0.00013377368,0.0000044584967],"about_ca_topic_score_codex":0.01515065,"about_ca_topic_score_gemma":0.013972354,"teacher_disagreement_score":0.01515065,"about_ca_system_score_codex":0.00038820895,"about_ca_system_score_gemma":0.0001733437,"threshold_uncertainty_score":0.030124903},"labels":[],"label_agreement":null},{"id":"W2060147469","doi":"10.1088/0004-637x/795/2/161","title":"THE FACTORY AND THE BEEHIVE. II. ACTIVITY AND ROTATION IN PRAESEPE AND THE HYADES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; University of Arizona; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Princeton University","keywords":"Physics; Astrophysics; Open cluster; Metallicity; Rossby number; Stars; Luminosity; Spectral line; Stellar classification; Star cluster; Equivalent width; Astronomy; Galaxy; Emission spectrum","score_opus":0.006457770572337375,"score_gpt":0.21055559411249097,"score_spread":0.2040978235401536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060147469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99582666,0.00017186183,0.00043617224,0.000041347346,0.0000016588301,0.000006380851,0.0003168919,0.000007766262,0.0031912383],"genre_scores_gemma":[0.99692446,0.00012204931,0.0006095088,0.000014078265,0.0000017932882,0.00000654973,0.00063254096,0.0000058587457,0.0016831113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975795,0.000028170081,0.000008540472,0.00010506909,0.000046841214,0.00005343581],"domain_scores_gemma":[0.9990164,0.0002924328,0.0003216675,0.00017928884,0.00009600612,0.00009418799],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032171677,0.00013173009,0.00015948707,0.0009468438,0.00053724024,0.00087249395,0.00036807448,0.00016604195,0.0027527395],"category_scores_gemma":[0.0021041397,0.00014656357,0.00015871444,0.0010475991,0.0006954289,0.0012154834,0.0011571248,0.00038557258,0.00046009754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023019614,0.000033614087,0.9502895,0.000033277265,0.00006176955,0.00023468396,0.0027709736,0.00054346654,0.0037602275,0.002555599,0.0004220321,0.039064705],"study_design_scores_gemma":[0.0000027269032,0.00002623084,0.9961068,0.0000046662517,0.000007219633,0.00011826385,0.00064753613,0.00022531727,0.0003916693,0.00031606096,0.0021485074,0.0000050209505],"about_ca_topic_score_codex":0.010743815,"about_ca_topic_score_gemma":0.026074953,"teacher_disagreement_score":0.010743815,"about_ca_system_score_codex":0.0004038277,"about_ca_system_score_gemma":0.00020264971,"threshold_uncertainty_score":0.021362603},"labels":[],"label_agreement":null},{"id":"W2060236946","doi":"10.1086/430084","title":"Laboratory and Theoretical Simulation of 3.4 μm Spectra of Hydrocarbons in Interstellar Sources","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; University of Waterloo","funders":"","keywords":"Physics; Spectral line; Astrophysics; Astrochemistry; Interstellar medium; Molecular cloud; Amorphous carbon; Interstellar cloud; Carbon fibers; Amorphous solid; Cosmic dust; Molecule; Hydrocarbon; Absorption (acoustics); Spectral bands; Infrared; Infrared spectroscopy; Astronomy; Galaxy; Stars; Crystallography; Composite number; Chemistry; Materials science; Optics; Organic chemistry","score_opus":0.00415180322106518,"score_gpt":0.23746225950358207,"score_spread":0.2333104562825169,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060236946","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98995614,0.00005603849,0.0016729517,0.00017129,0.000011343165,0.00001438363,0.00041967013,0.00010530019,0.0075929854],"genre_scores_gemma":[0.99827075,0.000029296387,0.0009938629,0.000029490393,0.0000045696197,0.0000210241,0.00026322657,0.000019146424,0.00036872295],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999162,0.000015921712,0.0000025802894,0.000016375068,0.00001771273,0.000031148713],"domain_scores_gemma":[0.9995277,0.00022513617,0.000071852315,0.000035917335,0.00007148603,0.00006794224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021109912,0.00034838385,0.000289036,0.00040777714,0.0005160767,0.0004761728,0.00081942364,0.0007319312,0.0028491726],"category_scores_gemma":[0.0010512107,0.0002139208,0.00066321396,0.00040827502,0.0005094131,0.00042190394,0.00041063418,0.00061527244,0.00017457845],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014666733,0.000111377354,0.009358936,0.000028190649,0.000028976432,0.00018057204,0.000057486544,0.9824034,0.0027314392,0.0031955722,0.00054974604,0.0012076709],"study_design_scores_gemma":[0.000068014146,0.000037615144,0.004949862,0.0000048550883,0.000011624701,0.00002632841,0.000042542157,0.99308974,0.0006135797,0.00092272187,0.00022147149,0.000011685679],"about_ca_topic_score_codex":0.02931164,"about_ca_topic_score_gemma":0.009561237,"teacher_disagreement_score":0.02931164,"about_ca_system_score_codex":0.0016889771,"about_ca_system_score_gemma":0.0006291332,"threshold_uncertainty_score":0.058282018},"labels":[],"label_agreement":null},{"id":"W2060286270","doi":"10.1086/341266","title":"A Highly Ordered Faraday Rotation Structure in the Interstellar Medium","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Polarization (electrochemistry); Faraday effect; Interstellar medium; Magnetic field; Galactic plane; Electron; Polarimetry; Electron density; Cosmic dust","score_opus":0.01027517163963955,"score_gpt":0.2201520083667481,"score_spread":0.20987683672710855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060286270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99029106,0.00052237517,0.0011498196,0.0000408992,0.00000724353,0.000013822588,0.00036276467,0.00005248642,0.007559599],"genre_scores_gemma":[0.99744785,0.00015428747,0.0009655381,0.000013847311,0.000008432992,0.000004262871,0.00044215927,0.000004932751,0.00095870154],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999207,0.0000024635003,0.000001600322,0.000016959582,0.000025940948,0.000032321615],"domain_scores_gemma":[0.99989855,0.0000062493823,0.000027154701,0.000008851629,0.000022723423,0.000036448626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000027386917,0.00021297586,0.00010606798,0.00093334896,0.00060270383,0.00080393424,0.00024918167,0.00014148405,0.00084059173],"category_scores_gemma":[0.00011842685,0.00012321257,0.00007532661,0.00072117435,0.00043391393,0.00023744209,0.00040928976,0.00013685001,0.00016929916],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028076497,0.000073685405,0.18242916,0.00012924756,0.00005983598,0.0041650007,0.0012311519,0.003736642,0.76661426,0.0064213863,0.0014049609,0.033453953],"study_design_scores_gemma":[0.000035785724,0.000146261,0.9385493,0.000022263768,0.00004599687,0.0023146465,0.0009433505,0.004291,0.03609546,0.0021633566,0.015324536,0.000067967296],"about_ca_topic_score_codex":0.030994158,"about_ca_topic_score_gemma":0.050133545,"teacher_disagreement_score":0.030994158,"about_ca_system_score_codex":0.0005479604,"about_ca_system_score_gemma":0.00041660687,"threshold_uncertainty_score":0.061627507},"labels":[],"label_agreement":null},{"id":"W2060320018","doi":"10.1086/497387","title":"Stellar Model Analysis of the Oscillation Spectrum of η Bootis Obtained from<i>MOST</i>","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université du Québec à Montréal; University of British Columbia; Université de Montréal; Saint Mary's University","funders":"","keywords":"Physics; Overtone; Astrophysics; Photometry (optics); Oscillation (cell signaling); Stars; Effective temperature; Spectral line; Astronomy","score_opus":0.009018494920630607,"score_gpt":0.21313099924424028,"score_spread":0.20411250432360967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060320018","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9845708,0.00005428404,0.009105013,0.00004907691,0.000008476952,0.0000065792738,0.00039823123,0.0002198906,0.0055877767],"genre_scores_gemma":[0.9979778,0.000018768762,0.0012551039,0.0000048195684,0.0000016391737,0.0000037971313,0.00028495153,0.000028643462,0.00042444497],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99997497,0.0000052229943,0.0000011733613,0.000010397234,0.00000412633,0.0000040843406],"domain_scores_gemma":[0.9999317,0.000022553162,0.000010087004,0.000010031498,0.000013920131,0.000011633845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010791478,0.00020990471,0.0001453551,0.00020225147,0.00019023655,0.00030506114,0.00021704532,0.00020896,0.0021037043],"category_scores_gemma":[0.00024455274,0.00007012321,0.00033988,0.0001379462,0.00009879437,0.00016504372,0.00014581835,0.00016231752,0.00037770887],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000694784,0.00020147646,0.14318389,0.00013539512,0.0002553709,0.0003604416,0.0005413176,0.7442016,0.06325336,0.01309518,0.003906111,0.030171055],"study_design_scores_gemma":[0.00002355983,0.0000434067,0.03978763,0.000004062085,0.000021318623,0.00006441197,0.000071995724,0.95593035,0.0017322623,0.0014598022,0.00085172,0.000009492434],"about_ca_topic_score_codex":0.006225368,"about_ca_topic_score_gemma":0.004728535,"teacher_disagreement_score":0.006225368,"about_ca_system_score_codex":0.00034441325,"about_ca_system_score_gemma":0.0001343124,"threshold_uncertainty_score":0.012378275},"labels":[],"label_agreement":null},{"id":"W2060367466","doi":"10.1088/0004-637x/708/2/1507","title":"COSMIC EVOLUTION OF BLACK HOLES AND SPHEROIDS. IV. THE<i>M</i><sub>BH</sub>-<i>L</i><sub>sph</sub>RELATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Alfred P. Sloan Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Luminosity; Galaxy; Redshift; Quasar; Active galactic nucleus; Galaxy formation and evolution; Black hole (networking); Accretion (finance); Astronomy; Stellar mass; Star formation","score_opus":0.004910888603713278,"score_gpt":0.19003031810595508,"score_spread":0.1851194295022418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060367466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99653566,0.00034648008,0.00024945708,0.000033823897,0.0000028985555,0.0000029114103,0.00025257966,0.000019167339,0.0025571191],"genre_scores_gemma":[0.9988049,0.00012013957,0.0002288885,0.000008305899,0.0000064198753,0.0000017476336,0.00035943408,0.0000063326224,0.00046379396],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999176,0.000015212431,0.0000059223967,0.00002367906,0.00001758521,0.000019902152],"domain_scores_gemma":[0.999491,0.00007294433,0.00022667927,0.00007585025,0.000046376055,0.000087184446],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001823586,0.00018032402,0.00007343662,0.0008331081,0.00025261845,0.0005324183,0.00012948185,0.00019541981,0.0011491412],"category_scores_gemma":[0.00081039,0.00009209914,0.00018016847,0.0005911779,0.00037889156,0.0002804523,0.0003480283,0.00018194369,0.00023923344],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008139652,0.000016061498,0.96954006,0.000017291724,0.00003448607,0.00017048245,0.00036926637,0.0005184698,0.009731318,0.0021612141,0.00029131153,0.017068688],"study_design_scores_gemma":[9.77651e-7,0.000011196307,0.99804187,0.0000019256609,0.00000710231,0.00013191777,0.00002732525,0.00036934568,0.00065688987,0.00019341877,0.0005560607,0.0000019102597],"about_ca_topic_score_codex":0.0039013824,"about_ca_topic_score_gemma":0.006745217,"teacher_disagreement_score":0.0039013824,"about_ca_system_score_codex":0.00042869896,"about_ca_system_score_gemma":0.00007882916,"threshold_uncertainty_score":0.0077573657},"labels":[],"label_agreement":null},{"id":"W2060407339","doi":"10.1088/0004-637x/715/1/51","title":"OBSERVATIONS OF DOPPLER BOOSTING IN KEPLER LIGHT CURVES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":182,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Brightness; Light curve; White dwarf; Amplitude; Radial velocity; Doppler effect; Primary (astronomy); Stars; Effective temperature; Astronomy; Photometry (optics); Mass ratio; Optics","score_opus":0.018983914824462513,"score_gpt":0.23695560231630552,"score_spread":0.217971687491843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060407339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870046,0.00031342596,0.002076468,0.00004849889,0.000018939587,0.000013389077,0.00033975922,0.00027394417,0.009910951],"genre_scores_gemma":[0.9982645,0.00010479264,0.0007734043,0.000017899243,0.000012981936,0.0000037240613,0.00021232039,0.000024049634,0.0005863984],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998167,0.00001815035,0.0000097792845,0.000054406377,0.00006338533,0.000037543137],"domain_scores_gemma":[0.9989361,0.0002187598,0.0003262021,0.00014172526,0.00022455468,0.00015261093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024132502,0.00022893693,0.00026298445,0.0013888355,0.00028846916,0.00049030886,0.00018800238,0.00027357115,0.0011047943],"category_scores_gemma":[0.0017627445,0.00017810616,0.00014057446,0.0008025224,0.0002334831,0.00028960255,0.00048327012,0.00035761204,0.00071713707],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038029527,0.000060428843,0.7210748,0.000086084416,0.00006241786,0.00054035906,0.0011343475,0.0013520666,0.2240289,0.00095786585,0.0014675418,0.048854962],"study_design_scores_gemma":[0.000005376772,0.000055728087,0.9827822,0.000011837187,0.00001812305,0.0007678721,0.000093434464,0.0012366859,0.010545381,0.00031095618,0.004151384,0.000021137637],"about_ca_topic_score_codex":0.0009510272,"about_ca_topic_score_gemma":0.0014012795,"teacher_disagreement_score":0.0013888355,"about_ca_system_score_codex":0.00029869453,"about_ca_system_score_gemma":0.00008978493,"threshold_uncertainty_score":0.0036959052},"labels":[],"label_agreement":null},{"id":"W2060478297","doi":"10.1086/321478","title":"Emissivity Statistics in Turbulent Compressible Magnetohydrodynamic Flows and the Density‐Velocity Correlation","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Emissivity; Turbulence; Magnetohydrodynamics; Computational physics; Position (finance); Magnetohydrodynamic drive; Magnetohydrodynamic turbulence; Thermal velocity; Flow velocity; Mechanics; Flow (mathematics); Plasma; Optics","score_opus":0.004661433973885264,"score_gpt":0.21253078307625903,"score_spread":0.20786934910237376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060478297","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98021543,0.00007342803,0.019043736,0.000046678415,0.0000037637142,0.000006611385,0.00006860275,0.000078467565,0.00046332987],"genre_scores_gemma":[0.99830085,0.00004399312,0.0014509227,0.00000365383,0.0000051852066,0.0000041042467,0.000110306595,0.000013471751,0.00006752515],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99977857,0.000061054576,0.000013815671,0.000042644395,0.000056336787,0.000047504393],"domain_scores_gemma":[0.9936935,0.0041369926,0.00114929,0.00043779812,0.00042369543,0.00015882081],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013786061,0.00029692423,0.00023347151,0.0012415928,0.00025425092,0.00063852867,0.00041870566,0.00028104064,0.0002485273],"category_scores_gemma":[0.011751598,0.00022977206,0.00014690509,0.00065234693,0.0009191481,0.0009490706,0.00047006967,0.00031322025,0.000052926483],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096275646,0.00018963983,0.2479301,0.00012563796,0.0001262268,0.00049420143,0.0006372845,0.62646484,0.050899666,0.045105916,0.00051179784,0.02655194],"study_design_scores_gemma":[0.00001954869,0.00006281118,0.06316831,0.000009439498,0.000012282027,0.00014204347,0.000054592434,0.9145157,0.013761222,0.007982603,0.00023450969,0.00003698862],"about_ca_topic_score_codex":0.0012966173,"about_ca_topic_score_gemma":0.0005259391,"teacher_disagreement_score":0.0013786061,"about_ca_system_score_codex":0.0003614467,"about_ca_system_score_gemma":0.00026152772,"threshold_uncertainty_score":0.0072908998},"labels":[],"label_agreement":null},{"id":"W2060696932","doi":"10.1086/318686","title":"Observational Constraints on Higher Order Clustering up to<i>z</i>≃ 1","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy; Dark matter; Correlation function (quantum field theory); Cosmic variance; Scaling; Skewness; Gaussian; Statistics; Quantum mechanics","score_opus":0.024466430692342278,"score_gpt":0.24452550396314734,"score_spread":0.22005907327080507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060696932","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931058,0.0001505454,0.0012713255,0.00008720365,0.0000033284973,0.000004449364,0.0005746296,0.0001136048,0.004689245],"genre_scores_gemma":[0.9985073,0.00006454111,0.00051836926,0.000023547278,0.00000803252,0.0000031848301,0.00063330994,0.00001504045,0.00022669775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967813,0.00003061286,0.00001569935,0.00007355082,0.00005431051,0.00014760706],"domain_scores_gemma":[0.9947131,0.0016709166,0.0018263233,0.00070568983,0.00039115825,0.00069265097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062735187,0.00027788628,0.00031932897,0.0013746638,0.00067818206,0.0009847155,0.0004233061,0.0003665319,0.0024190778],"category_scores_gemma":[0.003465715,0.00032800087,0.00032710558,0.00094876636,0.0006573764,0.0006658482,0.0007166014,0.0005893579,0.00057329907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000240347,0.00007445425,0.9451262,0.000070526294,0.000042657324,0.00016826067,0.0006438684,0.0063437875,0.020217337,0.009171183,0.0009676248,0.016933827],"study_design_scores_gemma":[0.000006748924,0.000032964497,0.98969704,0.00001494213,0.0000151973645,0.00010707718,0.000091540984,0.0034683645,0.0019067085,0.0032252895,0.0014163306,0.000017735252],"about_ca_topic_score_codex":0.009357596,"about_ca_topic_score_gemma":0.014592112,"teacher_disagreement_score":0.009357596,"about_ca_system_score_codex":0.0007556331,"about_ca_system_score_gemma":0.00032913167,"threshold_uncertainty_score":0.018606246},"labels":[],"label_agreement":null},{"id":"W2060716710","doi":"10.1086/426963","title":"Correlated Infrared and X-Ray Flux Changes Following the 2002 June Outburst of the Anomalous X-Ray Pulsar 1E 2259+586","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Infrared; Flux (metallurgy); Neutron star; Observatory; X-ray; X-ray pulsar; Afterglow; Magnetosphere; Astronomy; Far infrared; Gamma-ray burst; Plasma; Optics; Nuclear physics","score_opus":0.009059583907778572,"score_gpt":0.26534603511604354,"score_spread":0.256286451208265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060716710","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994665,0.000031827087,0.000046495235,0.000007997259,0.0000023897765,0.0000022452912,0.0000976403,0.0000070857595,0.00033781695],"genre_scores_gemma":[0.9989452,0.000044068016,0.00012950026,0.000015721509,0.0000071030186,0.0000048459865,0.00048653525,0.0000042785055,0.00036278588],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999429,0.000006841564,0.000004729202,0.00001649016,0.000015057393,0.000013946784],"domain_scores_gemma":[0.9995432,0.000049300656,0.00022984961,0.000026949197,0.00007947876,0.00007129705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013225494,0.00018321122,0.0002687128,0.0004501735,0.00022156654,0.00041656717,0.00014307667,0.00019232761,0.0004970372],"category_scores_gemma":[0.00068187714,0.0000992833,0.00013672949,0.0002866922,0.00015166886,0.00016293982,0.00026669417,0.00033262838,0.00016620621],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013759916,0.0002991235,0.86844194,0.00005735726,0.0001008152,0.0008064878,0.00045526185,0.0007361283,0.11349494,0.0001470222,0.00047178418,0.013613202],"study_design_scores_gemma":[0.0000037234756,0.000068172514,0.99758124,0.0000017017215,0.000009148325,0.00011458776,0.000037638747,0.00020797124,0.0017873282,0.000013439643,0.00017215265,0.0000027524347],"about_ca_topic_score_codex":0.002074155,"about_ca_topic_score_gemma":0.0040808367,"teacher_disagreement_score":0.002074155,"about_ca_system_score_codex":0.000178053,"about_ca_system_score_gemma":0.00006239441,"threshold_uncertainty_score":0.004124224},"labels":[],"label_agreement":null},{"id":"W2060747038","doi":"10.1088/0004-637x/795/1/44","title":"COSMOLOGICAL CONSTRAINTS FROM MEASUREMENTS OF TYPE Ia SUPERNOVAE DISCOVERED DURING THE FIRST 1.5 yr OF THE Pan-STARRS1 SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":343,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; National Central University; Ministerio de Ciencia, Tecnología e Innovación Productiva; Space Telescope Science Institute; Queen's University; Office of Science; Johns Hopkins University; Queen's University Belfast; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; U.S. Department of Energy; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Supernova; Astrophysics; Planck; Cosmic microwave background; Hubble's law; Light curve; Flatness (cosmology); Type (biology); Dark energy; Cosmological constant; Stars; Cosmology; Mathematical physics; Quantum mechanics","score_opus":0.025820129465537158,"score_gpt":0.2387430763720593,"score_spread":0.21292294690652214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060747038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99788266,0.00017100443,0.00016926735,0.000016589427,0.0000020532082,0.0000025589554,0.0010919127,0.00001190835,0.0006519804],"genre_scores_gemma":[0.99660957,0.000122027144,0.00027579902,0.000009561097,0.000007070055,0.000004649111,0.0027369643,0.000005368002,0.00022896878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999739,0.000049194674,0.000024582878,0.00007232259,0.00005797732,0.000057011606],"domain_scores_gemma":[0.99776936,0.00038258414,0.0011570733,0.00020888793,0.00020592182,0.00027622635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074425765,0.0002714029,0.0002394178,0.001131377,0.00028199021,0.00046613324,0.00024531217,0.00017992777,0.0011976879],"category_scores_gemma":[0.0028914297,0.00020260758,0.00034436482,0.00057010324,0.0001942554,0.00035056425,0.0007083785,0.00033255672,0.0002450188],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055805212,0.000009556975,0.99436426,0.000016294462,0.000037121816,0.000043639113,0.00005409807,0.00025388296,0.002482308,0.00007067497,0.0001277824,0.0024846517],"study_design_scores_gemma":[8.5691374e-7,0.000009238752,0.99937004,0.0000021614403,0.000007804473,0.000044428383,0.000017833092,0.00011743582,0.00016662749,0.0000086329,0.00025356584,0.000001441382],"about_ca_topic_score_codex":0.00982291,"about_ca_topic_score_gemma":0.02159126,"teacher_disagreement_score":0.00982291,"about_ca_system_score_codex":0.00033650277,"about_ca_system_score_gemma":0.00021229264,"threshold_uncertainty_score":0.019531488},"labels":[],"label_agreement":null},{"id":"W2060775020","doi":"10.1088/0004-637x/697/2/1269","title":"ZONAL FLOWS AND LONG-LIVED AXISYMMETRIC PRESSURE BUMPS IN MAGNETOROTATIONAL TURBULENCE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":388,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Turbulence; Magnetohydrodynamics; Advection; Rotational symmetry; Shearing (physics); Reynolds number; Pressure gradient; Inviscid flow; Magnetic diffusivity; Magnetohydrodynamic drive","score_opus":0.008807265165094056,"score_gpt":0.23373429478368227,"score_spread":0.2249270296185882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060775020","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99821836,0.000024770106,0.0014195736,0.000030578423,0.000004070398,0.000005471461,0.000033912493,0.000035217843,0.00022807728],"genre_scores_gemma":[0.9986424,0.000021730079,0.0011504182,0.0000054500747,0.0000028626273,0.0000067116002,0.000057631634,0.00000999829,0.00010278222],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999248,0.000022527147,0.0000048724783,0.000011414875,0.000013589567,0.00002280652],"domain_scores_gemma":[0.9993568,0.0002462468,0.00014483395,0.000050599643,0.00007895526,0.00012249348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044674822,0.00038050633,0.0003085086,0.00036520284,0.00045708648,0.0005647078,0.0003656808,0.000383676,0.00064555724],"category_scores_gemma":[0.0014441141,0.00026314647,0.0003498004,0.00029055894,0.00065018015,0.00044557167,0.00040712362,0.00040943397,0.000049627994],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045076368,0.00021234431,0.027921345,0.000044374454,0.00007323161,0.00028031188,0.00022946649,0.93937516,0.024180656,0.0044486322,0.00029373853,0.0024898532],"study_design_scores_gemma":[0.000027923124,0.000054815016,0.0032366859,0.0000028629647,0.0000059747317,0.000009090868,0.000015426907,0.99451435,0.0018225772,0.000257358,0.000046585632,0.0000063675097],"about_ca_topic_score_codex":0.008270749,"about_ca_topic_score_gemma":0.003919287,"teacher_disagreement_score":0.008270749,"about_ca_system_score_codex":0.0005246088,"about_ca_system_score_gemma":0.00046659517,"threshold_uncertainty_score":0.01644522},"labels":[],"label_agreement":null},{"id":"W2060824156","doi":"10.1086/497683","title":"Dust in the Host Galaxies of Supernovae","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy; Supernova; Luminosity; Astronomy; Luminous infrared galaxy; Population","score_opus":0.01161147856699053,"score_gpt":0.23254139923091702,"score_spread":0.2209299206639265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060824156","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99925095,0.0001753865,0.00005521145,0.0000048055235,0.0000018207714,0.0000018391377,0.00012844981,0.000008860807,0.00037257018],"genre_scores_gemma":[0.9993211,0.000084930565,0.00007605261,0.0000036195745,0.000005362466,0.0000015895062,0.0002916323,0.0000018766309,0.00021392346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998987,0.0000093599965,0.000009598022,0.000027552962,0.000022698321,0.000032086635],"domain_scores_gemma":[0.99961406,0.000042047464,0.00016941798,0.000026841044,0.000042291373,0.00010535215],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012941814,0.00017284922,0.00020181765,0.0011240606,0.00029224728,0.00057778327,0.0001916563,0.00014037044,0.0012133579],"category_scores_gemma":[0.00038227314,0.00015219577,0.00016879271,0.0005448093,0.00018749505,0.00017190346,0.0003558587,0.00010762939,0.00021160372],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047499227,0.00001779659,0.99025995,0.0000080381305,0.000027629745,0.00010604906,0.00008920973,0.00014231238,0.0066180713,0.000063740306,0.00006422565,0.002555468],"study_design_scores_gemma":[0.0000019288668,0.000023869818,0.9986363,0.0000019124184,0.000009325696,0.00013310989,0.00004204116,0.00016278337,0.0005988777,0.000027254782,0.00036131556,0.0000013261573],"about_ca_topic_score_codex":0.0037232472,"about_ca_topic_score_gemma":0.005962821,"teacher_disagreement_score":0.0037232472,"about_ca_system_score_codex":0.0002942325,"about_ca_system_score_gemma":0.000077306424,"threshold_uncertainty_score":0.0074031353},"labels":[],"label_agreement":null},{"id":"W2060871913","doi":"10.1088/0004-637x/757/2/179","title":"DISCOVERY OF AN ACTIVE SUPERMASSIVE BLACK HOLE IN THE BULGELESS GALAXY NGC 4561","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Supermassive black hole; Galaxy; Luminosity; Black hole (networking); Intermediate-mass black hole; Solar mass; Spectral line","score_opus":0.014709638812635949,"score_gpt":0.2487267857911567,"score_spread":0.23401714697852075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060871913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991756,0.00013775386,0.00009012132,0.000020978576,0.000004306317,0.000002324136,0.000038098966,0.000009380115,0.0005214454],"genre_scores_gemma":[0.99964166,0.000053953925,0.00012738993,0.000014188359,0.000004951291,0.0000010225931,0.000053098505,9.444173e-7,0.00010269645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998634,0.000008797373,0.00001191552,0.00004326075,0.00004088072,0.00003167944],"domain_scores_gemma":[0.9996666,0.000037085745,0.00010468734,0.000033961303,0.000024317156,0.00013343671],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020021132,0.0002140079,0.00031890217,0.0006280479,0.0004351674,0.0008090706,0.00026772878,0.00037776088,0.00095149665],"category_scores_gemma":[0.00038726264,0.00013387612,0.0001850577,0.0003127437,0.0004390719,0.00028065988,0.00080729625,0.00020155229,0.00024015902],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018906678,0.00008105043,0.92346495,0.000057013374,0.00007409923,0.0039051594,0.0016862688,0.00047369968,0.048703536,0.0010327442,0.00032835006,0.020003928],"study_design_scores_gemma":[0.000009180705,0.00018290925,0.9929178,0.000015276628,0.000034324654,0.0018441055,0.00043591572,0.0007859769,0.0018982143,0.00028165698,0.0015836551,0.000010949037],"about_ca_topic_score_codex":0.0032851277,"about_ca_topic_score_gemma":0.004733129,"teacher_disagreement_score":0.0032851277,"about_ca_system_score_codex":0.00026873025,"about_ca_system_score_gemma":0.00010826068,"threshold_uncertainty_score":0.0065320134},"labels":[],"label_agreement":null},{"id":"W2060879513","doi":"10.1088/0004-637x/781/1/45","title":"BLACK HOLE TRIPLE DYNAMICS: A BREAKDOWN OF THE ORBIT AVERAGE APPROXIMATION AND IMPLICATIONS FOR GRAVITATIONAL WAVE DETECTIONS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":212,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Gravitational wave; Binary black hole; Binary number; Eccentricity (behavior); Orbit (dynamics); Black hole (networking); LIGO; Chirp; Orbital decay","score_opus":0.011423691026681644,"score_gpt":0.28553532528921666,"score_spread":0.274111634262535,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060879513","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92930835,0.0005768679,0.06362268,0.0010601005,0.000048747763,0.00002896349,0.0002261004,0.00032010765,0.0048081335],"genre_scores_gemma":[0.99385566,0.00015311963,0.00546674,0.0000769032,0.000018920711,0.000016101318,0.000085756285,0.000058367496,0.0002683026],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99968696,0.000109199726,0.000015197438,0.000057179663,0.000071442206,0.00006009443],"domain_scores_gemma":[0.9966859,0.0020148426,0.000493362,0.0003847338,0.00019428295,0.00022691525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017488885,0.00040879785,0.0009677298,0.0005781055,0.0010041035,0.0012472788,0.0016068155,0.0011841384,0.0009600643],"category_scores_gemma":[0.010968532,0.00038157884,0.0006501262,0.00048091728,0.0012943883,0.0022812258,0.0009857373,0.0010489098,0.00011942798],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019802431,0.00007596063,0.04421119,0.000061470746,0.000100395955,0.0002924439,0.0002625746,0.8985956,0.0023790277,0.04123953,0.0006807398,0.011903121],"study_design_scores_gemma":[0.000011092814,0.000014679273,0.0016062412,0.0000065439617,0.0000064386986,0.000023762748,0.000021226875,0.9934546,0.00017718415,0.0045990585,0.00007235893,0.0000069492235],"about_ca_topic_score_codex":0.014915181,"about_ca_topic_score_gemma":0.0054401523,"teacher_disagreement_score":0.014915181,"about_ca_system_score_codex":0.00077402045,"about_ca_system_score_gemma":0.00090179255,"threshold_uncertainty_score":0.029656708},"labels":[],"label_agreement":null},{"id":"W2060908453","doi":"10.1086/339319","title":"The Mass‐to‐Light Function of Virialized Systems and the Relationship between Their Optical and X‐Ray Properties","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Mass-to-light ratio; Luminosity function; Halo; Luminosity; Galaxy; Baryon; Dark matter; Halo mass function; Mass ratio; Astronomy","score_opus":0.022012203623388696,"score_gpt":0.2004057248456542,"score_spread":0.17839352122226548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060908453","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99355984,0.00015183372,0.0027526882,0.000047855858,0.0000013922194,0.000003416402,0.00008948908,0.00003957689,0.0033539452],"genre_scores_gemma":[0.99900824,0.000053873686,0.00047468947,0.000006051831,0.0000037266868,0.0000042768543,0.00010379009,0.000009439597,0.0003361236],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989593,0.000022783775,0.0000056116537,0.000023974097,0.000017725382,0.000033987893],"domain_scores_gemma":[0.9983254,0.0005927208,0.0005449405,0.00016773642,0.00015350492,0.00021561624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044230066,0.00025144822,0.00013280036,0.001312609,0.0003063529,0.001086839,0.0003358518,0.00023141023,0.0019403315],"category_scores_gemma":[0.0023064348,0.00014534067,0.00022309324,0.0004918301,0.0004859373,0.00070076855,0.00056464376,0.00020241391,0.00041752963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006381455,0.000118416116,0.7669283,0.00010760276,0.00023670093,0.00039535138,0.0012466074,0.063625,0.053821154,0.07616243,0.0010572578,0.035663135],"study_design_scores_gemma":[0.000043746226,0.000287305,0.7353716,0.000035172,0.000078171564,0.0009417158,0.0004441388,0.217009,0.011654396,0.030692663,0.0033766185,0.000065504355],"about_ca_topic_score_codex":0.0015985972,"about_ca_topic_score_gemma":0.0007280344,"teacher_disagreement_score":0.0019403315,"about_ca_system_score_codex":0.00056463864,"about_ca_system_score_gemma":0.00012812078,"threshold_uncertainty_score":0.006491065},"labels":[],"label_agreement":null},{"id":"W2060925100","doi":"10.1088/0004-637x/731/1/47","title":"PHOTOMETRIC AND SPECTROSCOPIC EVOLUTION OF THE IIP SN 2007it TO DAY 944","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Ejecta; Astrophysics; Physics; Photometry (optics); Supernova; Flattening; Brightness; Pair-instability supernova; Radiative transfer; Spectral line; Luminosity; Emission spectrum; Astronomy; Light curve; Stars; Galaxy; Optics","score_opus":0.012588895115368324,"score_gpt":0.2197548764696142,"score_spread":0.20716598135424588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2060925100","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9916853,0.00011904284,0.0002715993,0.000035866684,0.000011176211,0.00001800687,0.0028961212,0.000050669594,0.004912211],"genre_scores_gemma":[0.98205805,0.00016611935,0.0007445752,0.000041449992,0.000023205195,0.000028716991,0.013376305,0.0000380463,0.0035235349],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988556,0.0000066380367,0.0000062667577,0.00003388976,0.00004622927,0.000021321417],"domain_scores_gemma":[0.9994941,0.000021473656,0.00012241081,0.000026150652,0.0002075945,0.00012833915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017321565,0.0003054759,0.00021545337,0.0015948436,0.00033155666,0.00052510086,0.00029118985,0.00027763628,0.0014547581],"category_scores_gemma":[0.00054232887,0.00014137373,0.00031212295,0.0008244751,0.00016843194,0.00016590806,0.00043389096,0.0004250448,0.00088660745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041363298,0.00018574561,0.95711744,0.000029418949,0.00010352853,0.0006115677,0.00023355849,0.0012502021,0.019397529,0.00038322096,0.0037919418,0.01648223],"study_design_scores_gemma":[0.0000015645637,0.000040358984,0.9974667,0.0000027612173,0.000010565102,0.00026098668,0.000045175006,0.0004745601,0.0004263118,0.00002419054,0.0012427424,0.000004124109],"about_ca_topic_score_codex":0.024026439,"about_ca_topic_score_gemma":0.029072788,"teacher_disagreement_score":0.024026439,"about_ca_system_score_codex":0.0008231543,"about_ca_system_score_gemma":0.00019790453,"threshold_uncertainty_score":0.047773182},"labels":[],"label_agreement":null},{"id":"W2061007181","doi":"10.1086/344258","title":"Violence in the Dark Ages","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Metallicity; Physics; Galaxy; Astronomy; Dwarf galaxy; Star formation; Stars; Universe; Luminosity; Dark matter","score_opus":0.009341076575904066,"score_gpt":0.2086709639795983,"score_spread":0.19932988740369423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061007181","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83234704,0.0018320855,0.0086859595,0.005878288,0.00014717971,0.00004553301,0.0011315712,0.00017616834,0.14975618],"genre_scores_gemma":[0.9937332,0.00029700508,0.00045025238,0.00024890125,0.0000150558135,0.000012290026,0.000112321555,0.0000106779835,0.0051203487],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"not_applicable","domain_scores_codex":[0.9997539,0.00012474535,0.0000063644793,0.000040662635,0.000022207396,0.00005219174],"domain_scores_gemma":[0.9994679,0.00017615201,0.000091129885,0.0000665004,0.000038774328,0.00015954627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003975351,0.0001287908,0.00029354714,0.00034349022,0.0007518543,0.0014202116,0.00027197876,0.00059301336,0.011618879],"category_scores_gemma":[0.0030514188,0.00010033785,0.0002357145,0.00030762865,0.0008394335,0.0009766249,0.0010521249,0.00062352465,0.0007611242],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003066017,0.00011100889,0.13712412,0.000079483965,0.000060861916,0.0016075202,0.0029392208,0.038736474,0.00093678903,0.77584267,0.00994446,0.03231087],"study_design_scores_gemma":[0.00021269139,0.00019101295,0.05834853,0.00013816974,0.00006602641,0.0017783127,0.004579897,0.052057892,0.0011513777,0.75680035,0.12460724,0.00006856997],"about_ca_topic_score_codex":0.0030256766,"about_ca_topic_score_gemma":0.0030973784,"teacher_disagreement_score":0.011618879,"about_ca_system_score_codex":0.00081041275,"about_ca_system_score_gemma":0.00045334492,"threshold_uncertainty_score":0.038869023},"labels":[],"label_agreement":null},{"id":"W2061117566","doi":"10.1088/0004-637x/774/2/142","title":"THE DISCOVERY OF PERIODIC MODULATIONS IN THE OPTICAL SPECTRA OF GALAXIES, POSSIBLY DUE TO ULTRARAPID LIGHT BURSTS FROM THEIR MASSIVE CENTRAL BLACK HOLES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Pulsar; Galaxy; Spectral line; Redshift; Crab Pulsar; Fourier transform; Modulation (music); Spectral density","score_opus":0.008066614912904863,"score_gpt":0.25802347259060293,"score_spread":0.24995685767769807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061117566","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99834514,0.00017842797,0.0009519531,0.000029749399,0.000004338718,0.0000034884392,0.00007632402,0.000023259292,0.00038737548],"genre_scores_gemma":[0.99896467,0.00003516843,0.00076178694,0.0000075024577,0.000008471631,0.0000019016677,0.00008928123,0.0000025046154,0.00012871047],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998869,0.000019067016,0.00000793977,0.00003497689,0.000027018817,0.000024086974],"domain_scores_gemma":[0.99918336,0.00020758955,0.00040631116,0.0000885012,0.000047187452,0.000067119356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027668392,0.00013994172,0.000093955045,0.0011336041,0.00015760794,0.00030220978,0.00017685353,0.00021310302,0.0006069014],"category_scores_gemma":[0.0008774565,0.00013173625,0.00015971214,0.0007004347,0.0003134661,0.00021809229,0.00027054414,0.00016563492,0.00010836613],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046485645,0.00008001375,0.81218946,0.00008650708,0.00010448468,0.0008543566,0.0004380823,0.00034576838,0.14426063,0.00073461904,0.00028355667,0.040157564],"study_design_scores_gemma":[0.0000033415074,0.00007549629,0.99052036,0.0000028466686,0.00001881177,0.0005460579,0.00004494914,0.0005153992,0.007656224,0.00019617182,0.000415754,0.0000045820016],"about_ca_topic_score_codex":0.0002663717,"about_ca_topic_score_gemma":0.00043127412,"teacher_disagreement_score":0.0011336041,"about_ca_system_score_codex":0.00014635199,"about_ca_system_score_gemma":0.000046705118,"threshold_uncertainty_score":0.0020302534},"labels":[],"label_agreement":null},{"id":"W2061231038","doi":"10.1086/426079","title":"The Bimodal Galaxy Color Distribution: Dependence on Luminosity and Environment","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":675,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Astrophysics; Physics; Galaxy; Luminosity function; Luminosity; Astronomy; Population; Sky; Redshift; Surface brightness fluctuation; Elliptical galaxy; Galaxy group; Demography","score_opus":0.005723644729161882,"score_gpt":0.1929095871839704,"score_spread":0.18718594245480852,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061231038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99901915,0.000046020676,0.00011598154,0.0000143461475,5.304545e-7,0.0000017571073,0.00042386615,0.000019761843,0.00035853384],"genre_scores_gemma":[0.9992754,0.000022697614,0.000048801256,0.0000045778193,0.0000024018022,0.0000014929977,0.00050418294,0.0000065739096,0.00013384895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996942,0.000070109156,0.000012126485,0.000073582945,0.000046585243,0.00010338138],"domain_scores_gemma":[0.9980566,0.0005257099,0.0006385718,0.00023834508,0.00020478357,0.00033600855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044930345,0.00019864581,0.0002816643,0.0015514194,0.00015982291,0.00069663685,0.00025587124,0.0002805981,0.0025919578],"category_scores_gemma":[0.0020890038,0.0001477494,0.00033670102,0.0010591636,0.00046294372,0.00040119392,0.00057577895,0.00020227692,0.0008892548],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021559752,0.00002555092,0.98974997,0.00001244514,0.000045991397,0.0001040436,0.0001561026,0.0012875735,0.0028596376,0.00017402915,0.00028232287,0.0050867484],"study_design_scores_gemma":[0.000003065361,0.000023953227,0.99790585,0.0000016010258,0.000005977979,0.00010332663,0.00006672981,0.001464527,0.00019160984,0.000048277012,0.0001808201,0.000004271422],"about_ca_topic_score_codex":0.0061571132,"about_ca_topic_score_gemma":0.00477743,"teacher_disagreement_score":0.0061571132,"about_ca_system_score_codex":0.00027780203,"about_ca_system_score_gemma":0.000097065225,"threshold_uncertainty_score":0.012242496},"labels":[],"label_agreement":null},{"id":"W2061341074","doi":"10.1088/0004-637x/796/2/106","title":"A GLOBAL THREE-DIMENSIONAL RADIATION MAGNETO-HYDRODYNAMIC SIMULATION OF SUPER-EDDINGTON ACCRETION DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":434,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Radiative transfer; Accretion (finance); Outflow; Astrophysics; Advection; Radiative flux; Angular momentum; Computational physics; Mechanics; Classical mechanics; Meteorology; Optics; Quantum mechanics","score_opus":0.008753679307178476,"score_gpt":0.24069660947760474,"score_spread":0.23194293017042628,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061341074","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989082,0.0000637524,0.005679711,0.00016285319,0.000017934783,0.000030211468,0.00025623507,0.00014294201,0.004564485],"genre_scores_gemma":[0.9950761,0.00004661528,0.003908524,0.000054571905,0.0000074138943,0.000041021878,0.00025703746,0.000035682933,0.000573023],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999335,0.000019017349,0.0000031963916,0.000011485274,0.000011048294,0.00002170259],"domain_scores_gemma":[0.9996432,0.00013932989,0.000057094498,0.000022103797,0.000035520596,0.000102710044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002389733,0.0005231844,0.0004804495,0.00026176946,0.00041728752,0.0005074128,0.0007021948,0.00076780183,0.0012741721],"category_scores_gemma":[0.000700345,0.00024272063,0.00055797846,0.00032095241,0.00065865414,0.00033855668,0.0006009045,0.00054500694,0.00009869927],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014000133,0.000105509076,0.006295436,0.000021155172,0.00004294777,0.00019364455,0.00008768984,0.9862481,0.0035082079,0.0016052076,0.00020418447,0.0015478886],"study_design_scores_gemma":[0.00004825475,0.000050342845,0.0017372266,0.000003285782,0.000007711047,0.000013751344,0.000023553624,0.9972051,0.0003804329,0.00037425992,0.0001503304,0.0000057635493],"about_ca_topic_score_codex":0.00863345,"about_ca_topic_score_gemma":0.004416768,"teacher_disagreement_score":0.00863345,"about_ca_system_score_codex":0.0006960402,"about_ca_system_score_gemma":0.0005954913,"threshold_uncertainty_score":0.017166376},"labels":[],"label_agreement":null},{"id":"W2061346331","doi":"10.1088/0004-637x/764/1/37","title":"THEORETICAL EXPLANATION OF THE COSMIC-RAY PERPENDICULAR DIFFUSION COEFFICIENT IN THE NEARBY STARBURST GALAXY NGC 253","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Galaxy; Diffusion; Perpendicular; Value (mathematics)","score_opus":0.0044432379590811834,"score_gpt":0.19539295636120332,"score_spread":0.19094971840212213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061346331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.73129565,0.003365684,0.16623051,0.0027603884,0.00017928492,0.0000712707,0.000629253,0.0005197141,0.094948255],"genre_scores_gemma":[0.98922265,0.00097577414,0.0048949732,0.00008316491,0.00005932197,0.000042298572,0.00007864732,0.00004545949,0.0045977836],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99995255,0.000008784392,0.0000022250617,0.000013270374,0.000011557507,0.000011568688],"domain_scores_gemma":[0.9997911,0.00007237948,0.000038169546,0.000022385113,0.0000397022,0.000036296216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025342926,0.0003870761,0.00040215882,0.00087735796,0.00046040266,0.0006142711,0.0008714907,0.0006476621,0.0026774232],"category_scores_gemma":[0.0008290033,0.00019900658,0.0005030231,0.00038574173,0.00071477285,0.0007783314,0.00052562315,0.00045689524,0.0003222134],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051145526,0.00003253827,0.0049663913,0.0000912306,0.00001677569,0.0007122692,0.00019752019,0.11060899,0.009021649,0.86789423,0.0017524211,0.004654953],"study_design_scores_gemma":[0.000063105,0.000042547686,0.008718458,0.000039698913,0.000038183713,0.00059757725,0.0001247994,0.6519355,0.0012193233,0.33425382,0.0029124427,0.00005456878],"about_ca_topic_score_codex":0.0076518967,"about_ca_topic_score_gemma":0.0024456799,"teacher_disagreement_score":0.0076518967,"about_ca_system_score_codex":0.0011001889,"about_ca_system_score_gemma":0.000410533,"threshold_uncertainty_score":0.015214741},"labels":[],"label_agreement":null},{"id":"W2061408873","doi":"10.1086/318060","title":"NGC 1333—Protostars, Dust Shells, and Triggered Star Formation","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Physics; Astrophysics; Star formation; Outflow; Brown dwarf; Molecular cloud; Astronomy; Cosmic dust; Population; Low Mass; Stars","score_opus":0.012812943173985068,"score_gpt":0.23385767963634288,"score_spread":0.2210447364623578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061408873","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980192,0.00006881417,0.00013848564,0.000023092125,0.0000011330529,0.0000031424297,0.0004243626,0.000020889234,0.0013008078],"genre_scores_gemma":[0.99897563,0.00003403108,0.00024575763,0.000012191967,0.0000019247436,0.0000026203613,0.0004860024,0.0000041799203,0.00023768774],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999645,0.00000348483,0.000002022792,0.000007984215,0.000009671963,0.00001232031],"domain_scores_gemma":[0.9998142,0.000013782236,0.00008755014,0.0000132521745,0.0000134093325,0.000057701127],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006916212,0.00011416135,0.000093703355,0.00040324486,0.0003508849,0.00023170299,0.00010784792,0.00015643904,0.0014228806],"category_scores_gemma":[0.00014873051,0.00006846196,0.0001223623,0.0007081513,0.00016400238,0.00012528493,0.00024187144,0.00013749354,0.0002320149],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023645499,0.00004485786,0.9655272,0.000022618007,0.00001986823,0.00088081794,0.0002873471,0.0004123184,0.023647593,0.00027679713,0.0008360443,0.0078080175],"study_design_scores_gemma":[0.0000023864884,0.000011001028,0.9982932,0.0000021498265,0.0000037320262,0.00048355068,0.00005301479,0.0001581999,0.0003972206,0.00007347681,0.00052027934,0.0000018159169],"about_ca_topic_score_codex":0.03166708,"about_ca_topic_score_gemma":0.06361735,"teacher_disagreement_score":0.03166708,"about_ca_system_score_codex":0.00047675212,"about_ca_system_score_gemma":0.00016478458,"threshold_uncertainty_score":0.06296551},"labels":[],"label_agreement":null},{"id":"W2061437502","doi":"10.1088/0004-637x/697/2/1439","title":"THE STELLAR DISK OF M81","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Galaxy; Stellar collision; Star formation; Thick disk; Main sequence; Spiral galaxy; K-type main-sequence star","score_opus":0.008533632610051535,"score_gpt":0.2653279702627846,"score_spread":0.2567943376527331,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061437502","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978339,0.00019010829,0.00004936268,0.000009438749,0.0000010383598,0.0000026961068,0.0002265263,0.000008680776,0.0016783015],"genre_scores_gemma":[0.99795675,0.00015094684,0.0002534046,0.000015205393,0.0000058139194,0.0000039187257,0.00087292335,0.0000041647245,0.00073673035],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993217,0.0000039997503,0.000005034525,0.000024904662,0.000016596743,0.000017297793],"domain_scores_gemma":[0.99987674,0.000009395528,0.000042102653,0.000014317482,0.000031288695,0.000026156573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009632738,0.00012799587,0.00014202418,0.0005779248,0.00038848547,0.00028530732,0.00014025807,0.00021656409,0.001146184],"category_scores_gemma":[0.00027765453,0.00008867717,0.00006838255,0.0005492428,0.00012909314,0.00028849364,0.0003212751,0.000065795335,0.0008141576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038851032,0.00007047184,0.817003,0.00013920716,0.00004863027,0.0011011966,0.0018157472,0.0009103263,0.13917306,0.00070150284,0.0023151636,0.036333174],"study_design_scores_gemma":[0.000003889056,0.00003820754,0.9960407,0.000005167146,0.000004766899,0.00029915417,0.0001315349,0.00025767757,0.0009898733,0.00004118569,0.0021847088,0.0000030293434],"about_ca_topic_score_codex":0.0044792662,"about_ca_topic_score_gemma":0.004960555,"teacher_disagreement_score":0.0044792662,"about_ca_system_score_codex":0.00041289732,"about_ca_system_score_gemma":0.00012383542,"threshold_uncertainty_score":0.008906364},"labels":[],"label_agreement":null},{"id":"W2061608768","doi":"10.1086/338352","title":"Inclusion of Turbulence in Solar Modeling","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Turbulence; Adiabatic process; Turbulence kinetic energy; K-epsilon turbulence model; K-omega turbulence model; Kinetic energy; Turbulence modeling","score_opus":0.01076740324992158,"score_gpt":0.21635592829953404,"score_spread":0.20558852504961245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061608768","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.25202355,0.001195542,0.7248817,0.00096516387,0.00050268066,0.00010360511,0.00020805761,0.0012674578,0.018852249],"genre_scores_gemma":[0.92094773,0.0007372736,0.07526676,0.00011131198,0.00016828603,0.000089057394,0.000082173356,0.00020643054,0.0023908815],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997365,0.00009347547,0.000017973,0.000026916905,0.00008508872,0.000039994542],"domain_scores_gemma":[0.9995901,0.00014313821,0.000059674123,0.00010642832,0.000059776365,0.000040770352],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004609894,0.0005803641,0.0005407445,0.00046285786,0.0005944799,0.00089132116,0.00067209173,0.0005829958,0.0007617779],"category_scores_gemma":[0.001635567,0.00031178122,0.001040895,0.00041339942,0.0005402165,0.0012105071,0.0011996941,0.0009290184,0.00018486263],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007468686,0.000048518763,0.003986062,0.00007772985,0.00005361291,0.00019644517,0.00015763586,0.85606146,0.011738985,0.102519244,0.00054039044,0.024545195],"study_design_scores_gemma":[0.000019849505,0.000029883437,0.0007694885,0.000011755609,0.000013263313,0.000035761495,0.000012033306,0.98110455,0.0016908442,0.014529627,0.0017625453,0.000020368589],"about_ca_topic_score_codex":0.0059752185,"about_ca_topic_score_gemma":0.0034324718,"teacher_disagreement_score":0.0059752185,"about_ca_system_score_codex":0.000646385,"about_ca_system_score_gemma":0.00085550116,"threshold_uncertainty_score":0.011880875},"labels":[],"label_agreement":null},{"id":"W2061645478","doi":"10.1086/424873","title":"Large-Scale Systematic Signals in Weak Lensing Surveys","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Weak gravitational lensing; Amplitude; Cosmology; Physics; SIGNAL (programming language); Statistical physics; Extinction (optical mineralogy); Scale (ratio); Astrophysics; Computational physics; Optics; Computer science; Galaxy; Redshift; Quantum mechanics","score_opus":0.009333285050242444,"score_gpt":0.21796012425486172,"score_spread":0.20862683920461927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061645478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878055,0.000111662404,0.010244325,0.00024987268,0.000012871146,0.000021232592,0.0002245602,0.00012751699,0.0012025489],"genre_scores_gemma":[0.9983253,0.000044909597,0.0012601701,0.000024360867,0.0000043851383,0.000012246294,0.00011651006,0.000015413385,0.00019666635],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9994879,0.00024210577,0.000024758598,0.000108019274,0.000069548405,0.00006763982],"domain_scores_gemma":[0.99187624,0.005233643,0.0014833095,0.00048748247,0.00051166443,0.0004076974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029704266,0.0004940705,0.00041211318,0.00078747567,0.0004944955,0.000921262,0.00072112767,0.00084952207,0.0008471806],"category_scores_gemma":[0.021195117,0.0004590932,0.00042397913,0.00077515055,0.0010952224,0.0011283798,0.0008646515,0.000679104,0.00010971376],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014348957,0.00005611078,0.08549265,0.000039262897,0.00008507299,0.00017598223,0.00016785217,0.8934181,0.0022038263,0.013165882,0.00062856113,0.0044232076],"study_design_scores_gemma":[0.000049032707,0.00006421025,0.015385644,0.000008360737,0.000024926654,0.000033298944,0.000033757555,0.9777012,0.0006872461,0.0057852445,0.00020023354,0.00002684207],"about_ca_topic_score_codex":0.014742903,"about_ca_topic_score_gemma":0.011557888,"teacher_disagreement_score":0.014742903,"about_ca_system_score_codex":0.0011193611,"about_ca_system_score_gemma":0.0005116043,"threshold_uncertainty_score":0.02931422},"labels":[],"label_agreement":null},{"id":"W2061662703","doi":"10.1086/592060","title":"The Nature of<i>p</i>‐Modes and Granulation in Procyon: New<i>MOST</i>Photometry and New Yale Convection Models","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université du Québec à Montréal; University of British Columbia; Université de Montréal; Saint Mary's University","funders":"","keywords":"Physics; Amplitude; Astrophysics; Photometry (optics); Spectral density; Spectral line; Computational physics; Convection; Stars; Optics; Astronomy; Statistics; Meteorology","score_opus":0.013694628583803142,"score_gpt":0.2236877749491516,"score_spread":0.20999314636534847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061662703","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99704605,0.00006599247,0.001714302,0.000054470143,0.0000024199337,0.0000031632458,0.000083906205,0.000051058625,0.0009786205],"genre_scores_gemma":[0.9984251,0.000039475497,0.0011624275,0.000010779226,0.000004761547,0.0000035753296,0.00014060162,0.00003687583,0.0001763896],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994695,0.000006931394,0.0000020275731,0.000022277149,0.000010006387,0.00001174677],"domain_scores_gemma":[0.9997495,0.000054077358,0.0000691087,0.000039754123,0.000017007045,0.00007045904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019904035,0.00025943885,0.00022758826,0.00033728738,0.00034591067,0.0007262425,0.00047371068,0.00026969274,0.00082257955],"category_scores_gemma":[0.00054354814,0.0003316531,0.00040927337,0.0002289983,0.0006009298,0.00047471284,0.0006737502,0.0004309889,0.00011090268],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060172967,0.00014757106,0.6182031,0.00011619939,0.00016964618,0.00088985957,0.0014007984,0.29470888,0.05704712,0.0077695176,0.001938778,0.017006848],"study_design_scores_gemma":[0.00007534774,0.00008054875,0.41107672,0.000023428956,0.000045723864,0.00031414928,0.00038743997,0.57808995,0.0055023488,0.003312474,0.0010367739,0.000055144465],"about_ca_topic_score_codex":0.010358611,"about_ca_topic_score_gemma":0.013681369,"teacher_disagreement_score":0.010358611,"about_ca_system_score_codex":0.0004972895,"about_ca_system_score_gemma":0.0002140871,"threshold_uncertainty_score":0.020596623},"labels":[],"label_agreement":null},{"id":"W2061671472","doi":"10.1088/0004-637x/798/2/118","title":"THE BINARY COMPANION OF YOUNG, RELATIVISTIC PULSAR J1906+0746","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Universities Space Research Association; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Centre National de la Recherche Scientifique; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; FP7 People: Marie-Curie Actions; National Science Foundation","keywords":"Pulsar; Physics; Neutron star; Binary pulsar; Astrophysics; White dwarf; Orbital period; Astronomy; Millisecond pulsar; Precession; Proper motion; Binary number; Stars","score_opus":0.022980108901226426,"score_gpt":0.32233415559745054,"score_spread":0.2993540466962241,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061671472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99769944,0.00029364476,0.00035966685,0.000016909033,0.000019570576,0.000009781729,0.00026831782,0.000022522418,0.0013100252],"genre_scores_gemma":[0.99810874,0.00014082796,0.0006018544,0.000014199592,0.000033178032,0.0000042133456,0.00069459074,0.0000051432858,0.00039715364],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979204,0.000017448965,0.00002003298,0.00006661243,0.000059203514,0.00004463251],"domain_scores_gemma":[0.9995765,0.00002506643,0.0002170429,0.00004335893,0.00004034465,0.000097635595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033702044,0.00022744942,0.00041948052,0.0007727514,0.0007823361,0.00067477475,0.0002485645,0.0002407232,0.0009279223],"category_scores_gemma":[0.00057645456,0.00012994853,0.00019997724,0.0007804106,0.00032025736,0.00038228586,0.00065291265,0.0002886981,0.000510977],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042805303,0.0002026376,0.9189687,0.00014702843,0.00008020822,0.0033595068,0.0008596896,0.00057271554,0.047231603,0.0013104208,0.0012506311,0.025588954],"study_design_scores_gemma":[0.000021181535,0.00047033397,0.9781531,0.000012568592,0.00004697586,0.006163832,0.00030372807,0.0009714896,0.00425831,0.00026693247,0.009314443,0.000016985821],"about_ca_topic_score_codex":0.0014928351,"about_ca_topic_score_gemma":0.0016794981,"teacher_disagreement_score":0.0014928351,"about_ca_system_score_codex":0.000242334,"about_ca_system_score_gemma":0.00020332537,"threshold_uncertainty_score":0.00310421},"labels":[],"label_agreement":null},{"id":"W2061683826","doi":"10.1088/0004-637x/799/1/33","title":"STATISTICAL ANALYSIS OF INTERFEROMETRIC MEASUREMENTS OF AXIS RATIOS FOR CLASSICAL Be STARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Monte Carlo method; Astrophysics; Stars; Interferometry; Line (geometry); Star (game theory); Thin disk; Optics; Computational physics; Statistics; Mathematics; Geometry","score_opus":0.06298642056134117,"score_gpt":0.2910246810468791,"score_spread":0.22803826048553794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061683826","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75749755,0.000112242924,0.24030568,0.00004069296,0.000014323505,0.000053396318,0.0004755895,0.00044789055,0.0010526237],"genre_scores_gemma":[0.9831039,0.0000305557,0.016102308,0.000008135953,0.000013512488,0.000034927103,0.0006144688,0.000022223217,0.00006990702],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9980907,0.0006084543,0.000118569136,0.0004923672,0.0006024155,0.00008745876],"domain_scores_gemma":[0.9871416,0.008691867,0.0018085138,0.0015287084,0.0006862786,0.00014300444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004156542,0.00034547233,0.00029762942,0.0022954077,0.00037817218,0.0006234323,0.0005705878,0.000257295,0.00063532474],"category_scores_gemma":[0.015586787,0.0002143984,0.00048225062,0.0009400715,0.00074198376,0.00073848595,0.00051312,0.00038037592,0.00015886902],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065478636,0.00020510859,0.71235764,0.0001290026,0.00083805126,0.00022983497,0.00036981338,0.08424852,0.04364565,0.011980741,0.0005435689,0.14479722],"study_design_scores_gemma":[0.000024911944,0.00042202318,0.45299903,0.000015622403,0.00013161235,0.0006638021,0.00016859696,0.5103422,0.021996722,0.011448017,0.00171492,0.00007249717],"about_ca_topic_score_codex":0.0006990796,"about_ca_topic_score_gemma":0.00071954326,"teacher_disagreement_score":0.004156542,"about_ca_system_score_codex":0.00044887193,"about_ca_system_score_gemma":0.00030824577,"threshold_uncertainty_score":0.021982193},"labels":[],"label_agreement":null},{"id":"W2061707236","doi":"10.1086/308477","title":"Globular Clusters in the Fornax Dwarf Spheroidal Galaxy","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Fornax Cluster; Dwarf spheroidal galaxy; Galaxy; Astronomy; Dwarf galaxy; Velocity dispersion; Dark matter; Interacting galaxy","score_opus":0.00897494303001944,"score_gpt":0.21922394707493756,"score_spread":0.21024900404491811,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061707236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963653,0.00029348346,0.00004697097,0.00021069768,0.000007013791,0.0000020596315,0.000028837145,0.0000059474546,0.003039764],"genre_scores_gemma":[0.9987155,0.00012076668,0.000051516643,0.00002487754,0.000007271953,8.6957846e-7,0.000043310676,7.5562605e-7,0.0010351695],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999641,0.0000045772535,0.000001304358,0.000011347767,0.0000060359334,0.0000125645465],"domain_scores_gemma":[0.99983454,0.000014130797,0.000054378972,0.000009513297,0.000023207293,0.0000641734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010284554,0.000063143336,0.00009338134,0.0004156114,0.0009649943,0.00071552803,0.00014071379,0.0003109391,0.001799536],"category_scores_gemma":[0.0003318609,0.000072112816,0.000044862834,0.0005226461,0.00060989906,0.00040087773,0.000465406,0.00011579461,0.00022078563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003416096,0.000047630067,0.90430576,0.00008796945,0.000039209663,0.0015990129,0.004842541,0.0021668568,0.015154715,0.043087445,0.004926723,0.023400443],"study_design_scores_gemma":[0.000021227015,0.000042323918,0.9816566,0.000019234669,0.000015899966,0.0004815735,0.0028169246,0.0010572618,0.00053724734,0.0060361535,0.0073052538,0.000010324425],"about_ca_topic_score_codex":0.040406603,"about_ca_topic_score_gemma":0.049636,"teacher_disagreement_score":0.040406603,"about_ca_system_score_codex":0.001258018,"about_ca_system_score_gemma":0.0004885701,"threshold_uncertainty_score":0.08034283},"labels":[],"label_agreement":null},{"id":"W2061717848","doi":"10.1086/379226","title":"The Hubble Constant from the Gravitational Lens B1608+6561","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"Consejo Nacional de Investigaciones Científicas y Técnicas; California Institute of Technology; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Galaxy; Hubble's law; Gravitational lens; Astrophysics; Lens (geology); Velocity dispersion; Einstein ring; Optics; Redshift","score_opus":0.009163109858514575,"score_gpt":0.2104719229204707,"score_spread":0.20130881306195614,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061717848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58178693,0.0016010907,0.37535554,0.0005718725,0.00015317432,0.000094511524,0.0024818736,0.0010815925,0.036873445],"genre_scores_gemma":[0.9716019,0.00051026914,0.01876445,0.00006452461,0.00007763546,0.00005276329,0.0016137994,0.00010175367,0.0072128465],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9997645,0.0000396723,0.000008809272,0.000054336186,0.00010571566,0.000026922717],"domain_scores_gemma":[0.9997408,0.00005104461,0.000060054008,0.00007401874,0.000041612955,0.00003247336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004596221,0.00075248786,0.00048049484,0.0005388175,0.00024487844,0.0006674023,0.0009976442,0.0005020916,0.0034849395],"category_scores_gemma":[0.0014750719,0.0003485981,0.00047338367,0.0004513511,0.00040597722,0.0011392523,0.0005947103,0.0005714241,0.0013839917],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002579931,0.000038819413,0.01758833,0.00014121117,0.00010515061,0.00026803534,0.00016167815,0.7806236,0.018470846,0.12055906,0.0042344453,0.057550855],"study_design_scores_gemma":[0.000067203364,0.00008062634,0.015416473,0.000030752773,0.00003569821,0.00017553236,0.000020931728,0.8871463,0.002061192,0.08386386,0.0110227745,0.00007864673],"about_ca_topic_score_codex":0.010631254,"about_ca_topic_score_gemma":0.0041663153,"teacher_disagreement_score":0.010631254,"about_ca_system_score_codex":0.00093765755,"about_ca_system_score_gemma":0.00074509607,"threshold_uncertainty_score":0.021138787},"labels":[],"label_agreement":null},{"id":"W2061733183","doi":"10.1086/429871","title":"An Automated Method for the Detection and Extraction of H<scp>i</scp>Self‐Absorption in High‐Resolution 21 Centimeter Line Surveys","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; University of Calgary","funders":"","keywords":"Physics; Amplitude; Brightness; Absorption (acoustics); Voxel; Pixel; Noise (video); Brightness temperature; Line (geometry); Hydrogen line; Astrophysics; Optics; Computational physics; Artificial intelligence; Computer science; Image (mathematics); Galaxy","score_opus":0.00973300709355599,"score_gpt":0.26262344919333014,"score_spread":0.2528904420997741,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061733183","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.09542668,0.000377,0.87106687,0.00031357937,0.00023616481,0.00045448387,0.004297404,0.022186447,0.0056414395],"genre_scores_gemma":[0.16296493,0.00014555987,0.8202633,0.00023337013,0.00013656309,0.00054844574,0.005287458,0.0006932862,0.0097271735],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99892396,0.00017397216,0.0000574634,0.00028114967,0.00046599383,0.000097463795],"domain_scores_gemma":[0.9973877,0.0005256149,0.00030622477,0.00051174103,0.0011401897,0.0001284634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001025483,0.00068544986,0.00061986496,0.0031716574,0.0011345326,0.001068343,0.0016506182,0.0012638603,0.0060094944],"category_scores_gemma":[0.0021967357,0.0007487579,0.00049651065,0.0015834777,0.00044934303,0.000728648,0.0007020078,0.0005319823,0.005112296],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003970425,0.00031950622,0.04304068,0.00025894496,0.00021153921,0.00023473195,0.00020923578,0.003774802,0.33545247,0.0014509414,0.030938834,0.5837113],"study_design_scores_gemma":[0.00034085644,0.00051902776,0.30356658,0.000049801933,0.00028688484,0.002338189,0.0002986703,0.24768943,0.36063904,0.004178324,0.07969562,0.0003976443],"about_ca_topic_score_codex":0.0044840486,"about_ca_topic_score_gemma":0.010883658,"teacher_disagreement_score":0.0060094944,"about_ca_system_score_codex":0.00040825538,"about_ca_system_score_gemma":0.0011530255,"threshold_uncertainty_score":0.020103753},"labels":[],"label_agreement":null},{"id":"W2061762764","doi":"10.1088/0004-637x/729/2/85","title":"GROWING MASSIVE BLACK HOLE PAIRS IN MINOR MERGERS OF DISK GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Mass ratio; Accretion (finance); Black hole (networking); Supermassive black hole; Orbital decay; Astronomy; Galaxy formation and evolution; Satellite","score_opus":0.011639833448073641,"score_gpt":0.20378838694653723,"score_spread":0.19214855349846358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061762764","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99770516,0.000065034306,0.00085031183,0.00010057995,0.00001077548,0.00001302999,0.00015503624,0.00005229278,0.0010477368],"genre_scores_gemma":[0.9980318,0.000041072923,0.0012133864,0.000054671298,0.000010882992,0.00001632919,0.0003263357,0.000020388317,0.0002851752],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998902,0.000027758846,0.0000049843443,0.00001993348,0.0000151998765,0.000041784857],"domain_scores_gemma":[0.9993291,0.00025288266,0.00009699832,0.000043148735,0.000061539395,0.0002163022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042681996,0.0005387366,0.00063417864,0.00058139605,0.00074429665,0.00084267004,0.0011246739,0.0009854533,0.0011417445],"category_scores_gemma":[0.0019914792,0.0004393495,0.0007825322,0.00035573103,0.00083196216,0.0005547151,0.0007565139,0.0007751442,0.000135388],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004398429,0.0003067335,0.059780143,0.000043331893,0.00019989362,0.00058498647,0.00021278199,0.9284365,0.0040038205,0.0030549224,0.00070248905,0.0022344599],"study_design_scores_gemma":[0.00012296512,0.00012488465,0.010276062,0.0000060188945,0.000030502171,0.00004445631,0.00010448215,0.98773164,0.00058927824,0.0006572507,0.00029919925,0.00001325431],"about_ca_topic_score_codex":0.021977175,"about_ca_topic_score_gemma":0.010885844,"teacher_disagreement_score":0.021977175,"about_ca_system_score_codex":0.0009939185,"about_ca_system_score_gemma":0.00080617965,"threshold_uncertainty_score":0.04369855},"labels":[],"label_agreement":null},{"id":"W2061805930","doi":"10.1086/430254","title":"Pulsations of the Oe Star ζ Ophiuchi from <i>MOST</i> Satellite Photometry and Ground-based Spectroscopy","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; St. Mary's University; University of Toronto; University of Victoria; Saint Mary's University; Dominion Astrophysical Observatory; University of British Columbia","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Asteroseismology; Light curve; Stars; Spectroscopy; Excited state; Opacity; Radial velocity; Astronomy; Overtone; Rotation period; Spectral line; Optics; Atomic physics","score_opus":0.008539851355598933,"score_gpt":0.22445850382703467,"score_spread":0.21591865247143574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061805930","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930346,0.00019166776,0.00012996202,0.00006982254,0.00002336635,0.000013649087,0.002421913,0.00002958122,0.0040854877],"genre_scores_gemma":[0.9902767,0.00021861019,0.00027883923,0.000041464176,0.000042288033,0.000008847653,0.006590618,0.000033376968,0.0025093008],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989724,0.0000071354916,0.000009470334,0.000022279972,0.000031852072,0.000032083437],"domain_scores_gemma":[0.99932754,0.00006624492,0.0001741155,0.00008642059,0.00020936025,0.0001363473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035442045,0.00022673272,0.00023993793,0.0014355431,0.0004139734,0.0006301846,0.00021251521,0.00024525978,0.0033777922],"category_scores_gemma":[0.0007908812,0.00011606556,0.00015258825,0.0010922748,0.0001374647,0.00028078488,0.00056098367,0.00021084586,0.0013149306],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010483218,0.000106497915,0.8879146,0.00020072723,0.00011007496,0.0009262933,0.0007494837,0.0004196341,0.054901633,0.00045486868,0.0048468313,0.048321024],"study_design_scores_gemma":[0.000010234864,0.000046316876,0.99384046,0.000008550929,0.000027939725,0.00013863674,0.00010542261,0.00011893791,0.002028114,0.000070769354,0.0035996912,0.0000047469794],"about_ca_topic_score_codex":0.0039327,"about_ca_topic_score_gemma":0.007323849,"teacher_disagreement_score":0.0039327,"about_ca_system_score_codex":0.00024436673,"about_ca_system_score_gemma":0.000209386,"threshold_uncertainty_score":0.011299849},"labels":[],"label_agreement":null},{"id":"W2061845540","doi":"10.1088/0004-637x/760/1/16","title":"THE DISTRIBUTION OF FAINT SATELLITES AROUND CENTRAL GALAXIES IN THE CANADA-FRANCE-HAWAII TELESCOPE LEGACY SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Astronomy; Luminosity function; Galaxy; Satellite galaxy; Milky Way; Luminosity; Luminous infrared galaxy","score_opus":0.008379501298705884,"score_gpt":0.20891680042458094,"score_spread":0.20053729912587506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061845540","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990977,0.000060893144,0.00003800676,0.000010401318,2.4356268e-7,0.0000015801588,0.0004390319,0.00000571722,0.00034645162],"genre_scores_gemma":[0.9987589,0.0000649945,0.00009846322,0.0000039009115,0.0000011591704,0.0000017226615,0.00088302616,0.0000021020194,0.00018565584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998796,0.000014891831,0.0000065976496,0.000033819724,0.000032694377,0.000032456257],"domain_scores_gemma":[0.9989778,0.00016218625,0.00025943256,0.00009903776,0.00029829337,0.00020320319],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024786705,0.00013140855,0.00013976982,0.0017061781,0.00041728356,0.00057002634,0.00034708547,0.00020674866,0.00094588305],"category_scores_gemma":[0.0011230953,0.00009767739,0.00019235365,0.0015936678,0.00038653132,0.00022737656,0.0004248844,0.000107702384,0.00010346199],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000028385706,0.000007001721,0.99480814,0.000008469062,0.000029554603,0.000057945563,0.00028696476,0.0008357114,0.0012344767,0.00015652139,0.00017479132,0.0023721016],"study_design_scores_gemma":[0.0000011151352,0.000003622913,0.99894816,0.0000018039632,0.000004959501,0.000026568066,0.000115807634,0.00063806097,0.00007775624,0.000010584103,0.00016840079,0.0000033149347],"about_ca_topic_score_codex":0.6122142,"about_ca_topic_score_gemma":0.70285577,"teacher_disagreement_score":0.3877858,"about_ca_system_score_codex":0.0020111057,"about_ca_system_score_gemma":0.0007796457,"threshold_uncertainty_score":0.7801391},"labels":[],"label_agreement":null},{"id":"W2061859185","doi":"10.1088/0004-637x/716/1/281","title":"NON-GAUSSIAN SCATTER IN CLUSTER SCALING RELATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Kurtosis; Skewness; Physics; Redshift; Gaussian; Scaling; Cluster (spacecraft); Statistical physics; Observable; Function (biology); Statistics; Astrophysics; Mathematics; Quantum mechanics; Galaxy","score_opus":0.00494796938068257,"score_gpt":0.21299792321049243,"score_spread":0.20804995382980987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061859185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9784727,0.0001268043,0.019891936,0.000115634364,0.000004955648,0.000012333249,0.00009725446,0.00008540552,0.0011929941],"genre_scores_gemma":[0.9991817,0.000018398478,0.000686097,0.0000062010627,0.000004102281,0.0000024284172,0.00004392055,0.0000080033715,0.0000492397],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99837446,0.0007165892,0.00007212242,0.00035081865,0.0002950678,0.0001909448],"domain_scores_gemma":[0.96834856,0.021495614,0.0048843534,0.003558869,0.0011311313,0.00058142305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004520108,0.00048950565,0.00038977904,0.0013378246,0.00048404952,0.0010512768,0.0005364277,0.00041749582,0.00080000696],"category_scores_gemma":[0.029156784,0.0002496935,0.0004647116,0.0011321235,0.0015395317,0.0012272181,0.0010946832,0.00056252757,0.00015798515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041763778,0.000075853546,0.7490545,0.000073873154,0.00033467068,0.000647806,0.0011894143,0.18301123,0.0072167017,0.039532285,0.0007246066,0.017721495],"study_design_scores_gemma":[0.000037386002,0.00011288237,0.31659022,0.000047111742,0.00007676781,0.00043300973,0.00040874167,0.62205666,0.00390715,0.055583857,0.00066178717,0.000084533465],"about_ca_topic_score_codex":0.005089947,"about_ca_topic_score_gemma":0.0047230134,"teacher_disagreement_score":0.005089947,"about_ca_system_score_codex":0.0006660593,"about_ca_system_score_gemma":0.0003480623,"threshold_uncertainty_score":0.02390486},"labels":[],"label_agreement":null},{"id":"W2061984469","doi":"10.1086/339899","title":"A 3.4 Micron Band in Magnesium Silicates: Preparation of Hydrocarbon-Silicate Condensates","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Silicate; Hydrocarbon; Absorption band; Physics; Amorphous solid; Methane; Absorption (acoustics); Infrared spectroscopy; Infrared; Interstellar medium; Forsterite; Spectral line; Analytical Chemistry (journal); Astrophysics; Mineralogy; Chemistry; Crystallography; Organic chemistry; Astronomy; Optics","score_opus":0.012015050467200177,"score_gpt":0.24040748133440965,"score_spread":0.22839243086720948,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061984469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99687284,0.00029025303,0.0016202118,0.000026223537,0.000009041271,0.00002535581,0.000080541104,0.000039711776,0.0010357614],"genre_scores_gemma":[0.9970688,0.0001974644,0.0016125225,0.00001588937,0.0000065352665,0.000015830807,0.000101989805,0.000022001419,0.00095894834],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998989,0.000013309205,0.0000060156112,0.000020750822,0.00003212755,0.00002889623],"domain_scores_gemma":[0.9998703,0.00003722087,0.000034066914,0.00001655435,0.000018328608,0.000023507639],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020986049,0.0002864687,0.00016405557,0.00034826377,0.00025514213,0.00013166529,0.00019864504,0.00017727562,0.0012145888],"category_scores_gemma":[0.0002542948,0.00015902348,0.0001338802,0.00019492517,0.00024947146,0.00012688844,0.00019563794,0.00022449793,0.00026322325],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042606902,0.000005641948,0.00017542734,0.000022835515,0.0000028239203,0.000023753173,0.000025246136,0.000052590927,0.9989976,0.00003740022,0.000007751135,0.00060628675],"study_design_scores_gemma":[0.000012610254,0.0001521613,0.0015653357,0.0000029465184,0.000005003495,0.000027662945,0.000014734996,0.00020367451,0.99734277,0.000029995157,0.0006409038,0.0000021643173],"about_ca_topic_score_codex":0.0008353338,"about_ca_topic_score_gemma":0.0026377146,"teacher_disagreement_score":0.0012145888,"about_ca_system_score_codex":0.00018144508,"about_ca_system_score_gemma":0.0001235837,"threshold_uncertainty_score":0.0040632486},"labels":[],"label_agreement":null},{"id":"W2061996623","doi":"10.1086/344638","title":"Viscous Diffusion and Photoevaporation of Stellar Disks","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":146,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Photoevaporation; Diffusion; Computational astrophysics; Stellar atmosphere; Viscous liquid; Stars; Stellar evolution","score_opus":0.008851767918445361,"score_gpt":0.23132569828577068,"score_spread":0.22247393036732532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2061996623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8075478,0.022996234,0.0031213858,0.019435385,0.01539497,0.0001403992,0.0012892988,0.00050843455,0.1295661],"genre_scores_gemma":[0.8707399,0.007563134,0.00067714305,0.0004520879,0.0045767394,0.000023752904,0.0008322348,0.00014452449,0.11499047],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99961567,0.00004099621,0.000018822886,0.00006647504,0.00019542164,0.00006258925],"domain_scores_gemma":[0.99681574,0.0006329861,0.00033983565,0.00017149097,0.001604611,0.00043535623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005479162,0.0002267617,0.00057524955,0.0009711301,0.0011438564,0.002269326,0.0007135971,0.0012078321,0.02732794],"category_scores_gemma":[0.0063433326,0.0002016907,0.00022445274,0.00061861373,0.0006039427,0.0014926055,0.0007850036,0.00038108657,0.0052799336],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0051372526,0.00040239125,0.07976748,0.004971535,0.00030755246,0.008629496,0.001971833,0.0073078084,0.14916176,0.049128346,0.31422344,0.37899116],"study_design_scores_gemma":[0.000501046,0.0009538462,0.33928666,0.00049686624,0.00022378395,0.004913071,0.002961537,0.028940689,0.08569247,0.053443663,0.48233294,0.00025352626],"about_ca_topic_score_codex":0.0008206391,"about_ca_topic_score_gemma":0.0008034583,"teacher_disagreement_score":0.02732794,"about_ca_system_score_codex":0.0005691919,"about_ca_system_score_gemma":0.0005791793,"threshold_uncertainty_score":0.09142101},"labels":[],"label_agreement":null},{"id":"W2062032999","doi":"10.1088/0004-637x/775/1/14","title":"DISCOVERY OF THE TRANSITION OF A MINI-BROAD ABSORPTION LINE INTO A BROAD ABSORPTION LINE IN THE SDSS QUASAR J115122.14+020426.3","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Astrophysics; Absorption spectroscopy; Physics; Blueshift; Spectral line; Absorption (acoustics); Sky; Line (geometry); Emission spectrum; Galaxy; Astronomy; Optics; Geometry","score_opus":0.0076665697744398385,"score_gpt":0.2179933071618233,"score_spread":0.21032673738738347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062032999","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99858654,0.00018461309,0.00025344413,0.00003176112,0.000010245533,0.000008189817,0.00016143202,0.000049751718,0.0007140949],"genre_scores_gemma":[0.999037,0.000036361416,0.00027541548,0.000038760827,0.000012760881,0.000004985133,0.000368508,0.0000050657577,0.00022118672],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989533,0.000005572485,0.0000061519527,0.000034577602,0.000029499677,0.000028920165],"domain_scores_gemma":[0.99956006,0.000026897658,0.00016564681,0.000036437606,0.00003616922,0.00017475961],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020179129,0.00026067882,0.00021716248,0.0009192282,0.0004617315,0.0006264473,0.00030419105,0.00060336164,0.000902546],"category_scores_gemma":[0.00038117162,0.00020085128,0.00021368577,0.00052356505,0.00031405987,0.00017868807,0.000552594,0.00044652753,0.0002446416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003350585,0.00021192907,0.6496045,0.00009455303,0.00015437735,0.006066394,0.0007940707,0.00021290164,0.3235992,0.0005332237,0.0010541425,0.017339641],"study_design_scores_gemma":[0.000010244618,0.0001954446,0.9910738,0.0000072863786,0.000030776777,0.0023693722,0.00013801303,0.00021260843,0.003824628,0.000064003296,0.0020627559,0.000011179614],"about_ca_topic_score_codex":0.0020497972,"about_ca_topic_score_gemma":0.0042573432,"teacher_disagreement_score":0.0020497972,"about_ca_system_score_codex":0.00024863277,"about_ca_system_score_gemma":0.000100098936,"threshold_uncertainty_score":0.0040757656},"labels":[],"label_agreement":null},{"id":"W2062221659","doi":"10.1088/0004-637x/761/1/20","title":"SIZE BIAS AND DIFFERENTIAL LENSING OF STRONGLY LENSED, DUSTY GALAXIES IDENTIFIED IN WIDE-FIELD SURVEYS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Galaxy; Astrophysics; Halo; Lens (geology); Millimeter; Magnification; Strong gravitational lensing; Weak gravitational lensing; Gravitational lens; Point source; Optics; Redshift","score_opus":0.017413795343577683,"score_gpt":0.22807977130498883,"score_spread":0.21066597596141115,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062221659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994479,0.000053729113,0.00026437268,0.000012933746,7.2336076e-7,9.478729e-7,0.000024074516,0.0000043282107,0.00019101582],"genre_scores_gemma":[0.99984884,0.000011242689,0.000066966044,0.0000037850918,0.0000018906094,5.368427e-7,0.000036933874,0.0000012965993,0.000028495195],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99912375,0.00023700992,0.00006462766,0.00029720645,0.00016056604,0.00011683678],"domain_scores_gemma":[0.98796695,0.0051129307,0.0046286876,0.0011814702,0.0005555162,0.0005543836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015181979,0.0002370953,0.00027102669,0.0015033016,0.00028112857,0.00058193965,0.00039834197,0.000350529,0.00086178386],"category_scores_gemma":[0.011653411,0.00020213773,0.00022588429,0.0006438534,0.00090819626,0.0008163891,0.00092591357,0.00018939642,0.00013688864],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054997818,0.0000062017994,0.99302834,0.000009305502,0.000046603807,0.00005635588,0.00014535156,0.0004410795,0.0036078668,0.00024039569,0.000033188287,0.002330305],"study_design_scores_gemma":[0.000003445164,0.000023814291,0.9964605,0.0000028413322,0.000022308159,0.00019926707,0.000119186094,0.0013190308,0.0014479931,0.00032535772,0.000072265,0.0000040183745],"about_ca_topic_score_codex":0.0022162641,"about_ca_topic_score_gemma":0.0036028703,"teacher_disagreement_score":0.0022162641,"about_ca_system_score_codex":0.0004647439,"about_ca_system_score_gemma":0.00011341614,"threshold_uncertainty_score":0.008029103},"labels":[],"label_agreement":null},{"id":"W2062294481","doi":"10.1086/528710","title":"The <i>Spitzer</i> Gould Belt Survey of Large Nearby Interstellar Clouds: Discovery of a Dense Embedded Cluster in the Serpens-Aquila Rift","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Serpens; Protostar; Cluster (spacecraft); Young stellar object; Line (geometry); Bow shock (aerodynamics); Interstellar medium","score_opus":0.015610504488321719,"score_gpt":0.25581061029966295,"score_spread":0.24020010581134124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062294481","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986582,0.00008254552,0.00006198585,0.000038160088,0.0000025993218,0.0000043938185,0.00018878719,0.000016510614,0.00094682735],"genre_scores_gemma":[0.99858713,0.00011779252,0.0003222854,0.000024219979,0.000010633061,0.000003975983,0.0005412765,0.0000042875,0.00038853782],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999422,0.0000037355605,0.0000024486678,0.000014894878,0.00001952888,0.000017087717],"domain_scores_gemma":[0.9998431,0.000009577018,0.00007217027,0.000016099093,0.000013224454,0.000045716202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010585549,0.00015436456,0.000090343434,0.0015045597,0.00031780495,0.00029543924,0.00023308517,0.000097423355,0.0010221978],"category_scores_gemma":[0.00024236013,0.00006618569,0.000078040524,0.00056163745,0.00036777603,0.00015473194,0.00045791527,0.000105029496,0.00020552026],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000090833906,0.000027729153,0.96274465,0.000028548566,0.000028328534,0.0007966272,0.00048822936,0.00019140616,0.01468671,0.0002361854,0.0014101305,0.019270543],"study_design_scores_gemma":[0.0000032842415,0.000011371862,0.99757916,0.000005343677,0.0000053014755,0.00034475097,0.00011737281,0.000113242495,0.00059684133,0.000032262105,0.0011893221,0.000001800986],"about_ca_topic_score_codex":0.0087067,"about_ca_topic_score_gemma":0.022485308,"teacher_disagreement_score":0.0087067,"about_ca_system_score_codex":0.00031978506,"about_ca_system_score_gemma":0.0001864004,"threshold_uncertainty_score":0.01731205},"labels":[],"label_agreement":null},{"id":"W2062323950","doi":"10.1086/377364","title":"On the Nature of the Ringlike Structure in the Outer Galactic Disk","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Satellite galaxy; Galaxy; Astronomy; Context (archaeology); Milky Way; Longitude; Thin disk; Latitude; Geology; Paleontology","score_opus":0.0043162006953772775,"score_gpt":0.20030508469365346,"score_spread":0.1959888839982762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062323950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930977,0.00015568465,0.0010422347,0.0002531382,0.0000062541685,0.000008768631,0.00012060199,0.000030602205,0.0052850186],"genre_scores_gemma":[0.99860734,0.00008799853,0.00068947044,0.00002835486,0.0000055083956,0.000003817112,0.00006887489,0.000021908221,0.00048679553],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99989855,0.00004453356,0.000002910024,0.000016744274,0.000012134377,0.000025090869],"domain_scores_gemma":[0.9990503,0.0003770888,0.00018438029,0.00007661517,0.00008346262,0.00022816073],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036837993,0.0002510831,0.0003833773,0.0004241681,0.0007580178,0.0012241073,0.0008297481,0.00067277526,0.003467987],"category_scores_gemma":[0.0026441792,0.0002975023,0.00029908266,0.0003922457,0.00092961563,0.001069084,0.0008459101,0.0005776429,0.00027893527],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074948516,0.00024681384,0.18988273,0.0001467245,0.00021678954,0.0016188492,0.002082656,0.72926396,0.019587686,0.044628415,0.0021871093,0.009388738],"study_design_scores_gemma":[0.00018284943,0.00021997603,0.110027075,0.000036856778,0.00007271237,0.00027205542,0.0013412298,0.8700193,0.0013721597,0.013325373,0.0030622089,0.00006809154],"about_ca_topic_score_codex":0.02058506,"about_ca_topic_score_gemma":0.018310793,"teacher_disagreement_score":0.02058506,"about_ca_system_score_codex":0.0009896598,"about_ca_system_score_gemma":0.0003445724,"threshold_uncertainty_score":0.04093051},"labels":[],"label_agreement":null},{"id":"W2062326041","doi":"10.1086/509636","title":"Escape of Ionizing Radiation from Star-forming Regions in Young Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Redshift; Galaxy; Cosmology; Radiative transfer; Star formation; Reionization; Background radiation; Galaxy formation and evolution","score_opus":0.006688970105285735,"score_gpt":0.19977358399954148,"score_spread":0.19308461389425574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062326041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989761,0.000028570987,0.00064506056,0.000011998181,6.907045e-7,0.0000017857667,0.00006748858,0.000022280516,0.0002460575],"genre_scores_gemma":[0.9991448,0.000024268285,0.00055978773,0.0000056726008,0.0000011012822,0.000002525449,0.00015735593,0.000008093954,0.000096364485],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999497,0.000010647042,0.0000028800287,0.00001268233,0.00000793724,0.000016176597],"domain_scores_gemma":[0.99950206,0.00019395852,0.00012962225,0.000042073796,0.00003910632,0.00009321945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034301047,0.00028063392,0.00022477057,0.00035694614,0.00024893542,0.00040174712,0.0004374908,0.00039034642,0.00048495794],"category_scores_gemma":[0.001585929,0.00020798143,0.00050522486,0.00032953825,0.00031433784,0.00037275103,0.00039583718,0.000277432,0.0000974858],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000241072,0.000053668537,0.30853578,0.000038706017,0.00010852368,0.00033399547,0.00023466068,0.67540246,0.009766206,0.0016648474,0.0001530009,0.0034670152],"study_design_scores_gemma":[0.00011281463,0.00012850814,0.20513168,0.00001368401,0.0000533694,0.00023537986,0.00010442647,0.7872353,0.004962997,0.0016322372,0.00036377268,0.000025829919],"about_ca_topic_score_codex":0.009716186,"about_ca_topic_score_gemma":0.005400432,"teacher_disagreement_score":0.009716186,"about_ca_system_score_codex":0.00059924566,"about_ca_system_score_gemma":0.0002090674,"threshold_uncertainty_score":0.019319236},"labels":[],"label_agreement":null},{"id":"W2062356233","doi":"10.1086/374333","title":"CO Molecular Gas in Infrared‐luminous Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":200,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Luminous infrared galaxy; Far infrared; Infrared; Line (geometry); Flux (metallurgy); Emission spectrum; Luminosity; Astronomy; Spectral line","score_opus":0.007249717911560777,"score_gpt":0.23091281062257696,"score_spread":0.22366309271101617,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062356233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995745,0.00009023109,0.000042775628,0.000006055146,5.7950916e-7,8.391403e-7,0.00012151153,0.0000060026123,0.00015756389],"genre_scores_gemma":[0.9995009,0.00006007883,0.00004072506,0.0000057337543,0.0000039094693,0.0000017127078,0.00032710258,0.0000016828117,0.000058177502],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998053,0.00002502234,0.000008444689,0.00006683004,0.00003341781,0.00006109157],"domain_scores_gemma":[0.9992643,0.00009395851,0.00030728205,0.0000665437,0.00008485271,0.00018309127],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023854262,0.00020965088,0.00029320587,0.001900599,0.00026120924,0.00059322227,0.00030195864,0.00021520062,0.0005974293],"category_scores_gemma":[0.0007016399,0.0001689908,0.00018419386,0.0011419577,0.00036521885,0.0002250296,0.00043415203,0.00015916121,0.0002915012],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036392437,0.000013113851,0.9962998,0.000004356674,0.000021897302,0.000029644343,0.00005540411,0.00010058446,0.0019030339,0.000030514237,0.00005022036,0.0014551291],"study_design_scores_gemma":[7.549024e-7,0.00001197303,0.9994093,9.5152694e-7,0.0000056640574,0.000045923978,0.00003442553,0.00025533707,0.00014758087,0.000012260153,0.00007471877,0.0000010844851],"about_ca_topic_score_codex":0.009045668,"about_ca_topic_score_gemma":0.0076089506,"teacher_disagreement_score":0.009045668,"about_ca_system_score_codex":0.00025240105,"about_ca_system_score_gemma":0.00011712601,"threshold_uncertainty_score":0.017986},"labels":[],"label_agreement":null},{"id":"W2062362017","doi":"10.1088/0004-637x/777/1/9","title":"REVEALING THE ASYMMETRY OF THE WIND OF THE VARIABLE WOLF-RAYET STAR WR1 (HD 4004) THROUGH SPECTROPOLARIZATION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"Polarization (electrochemistry); Asymmetry; Depolarization; Stokes parameters; Phase (matter); Spectral line; Emission spectrum","score_opus":0.007558158944766027,"score_gpt":0.20662167783058413,"score_spread":0.1990635188858181,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062362017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99533564,0.00025563609,0.0016552499,0.000038176346,0.000010619351,0.000007153516,0.00063084456,0.00005600113,0.0020107576],"genre_scores_gemma":[0.9965307,0.00014128358,0.0019474785,0.000020600059,0.00001672795,0.0000044376898,0.0008504578,0.000012690141,0.00047551177],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999341,0.000007241645,0.0000027658866,0.000021427351,0.00001852753,0.000016034332],"domain_scores_gemma":[0.9998462,0.00002929562,0.00005416983,0.00002038209,0.00002201676,0.000027937738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012518832,0.00013456262,0.00011873973,0.0008502177,0.00015835316,0.00027240356,0.00013200975,0.00019889315,0.0010534904],"category_scores_gemma":[0.0002046813,0.00011825318,0.00012718122,0.00035829982,0.000104725375,0.0002545029,0.00031795923,0.00022819836,0.00028500962],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040227533,0.00005622891,0.4883092,0.00011697918,0.0001082886,0.0008755777,0.00037112905,0.0010140411,0.4704215,0.0003409856,0.00057584443,0.037407964],"study_design_scores_gemma":[0.000009948282,0.00008219036,0.9811014,0.000009806854,0.00002424989,0.001009424,0.00017553083,0.0020417525,0.013433476,0.00024550266,0.0018553521,0.000011333688],"about_ca_topic_score_codex":0.00052200834,"about_ca_topic_score_gemma":0.0015934646,"teacher_disagreement_score":0.0010534904,"about_ca_system_score_codex":0.00010329588,"about_ca_system_score_gemma":0.00005571736,"threshold_uncertainty_score":0.0035242438},"labels":[],"label_agreement":null},{"id":"W2062506515","doi":"10.1086/424997","title":"Photometry of Irregular Satellites of Uranus and Neptune","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Neptune; Uranus; Jovian; Photometry (optics); Observatory; Solar System; Trans-Neptunian object","score_opus":0.0057197483957986215,"score_gpt":0.20141832779992103,"score_spread":0.1956985794041224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062506515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983374,0.000041263964,0.00009887861,0.0000045023667,0.0000013167258,0.0000076456045,0.00026047966,0.000010450552,0.0012379013],"genre_scores_gemma":[0.9981256,0.00003147181,0.0005235365,0.000006095925,0.0000025441373,0.000005573497,0.0009509177,0.0000062611584,0.0003480544],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984205,0.000023189525,0.000009108922,0.000043786586,0.00004952508,0.00003225613],"domain_scores_gemma":[0.99962795,0.0000351636,0.00008666367,0.00006779073,0.000076327255,0.000106115935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018209693,0.00020074885,0.00020505088,0.0010105709,0.00040317047,0.00024444878,0.00022400123,0.0001653851,0.00069637166],"category_scores_gemma":[0.00046366113,0.00012503848,0.00011951365,0.0007215219,0.00020930095,0.00015708568,0.00040082957,0.00013670081,0.00023683885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012735715,0.000035698293,0.9647039,0.000023441115,0.00002525972,0.00015214365,0.0010601793,0.0003007218,0.019714812,0.00007610176,0.00024255842,0.013537805],"study_design_scores_gemma":[0.0000022528104,0.000024435809,0.99849737,0.0000014008497,0.0000039942474,0.00012378512,0.000115667855,0.0001919587,0.0004340874,0.000011876443,0.00059156463,0.0000016645579],"about_ca_topic_score_codex":0.011064671,"about_ca_topic_score_gemma":0.027016755,"teacher_disagreement_score":0.011064671,"about_ca_system_score_codex":0.0003176535,"about_ca_system_score_gemma":0.00012120521,"threshold_uncertainty_score":0.022000551},"labels":[],"label_agreement":null},{"id":"W2062608889","doi":"10.1086/517960","title":"From Thin to Thick: The Impact of X‐Ray Irradiation on Accretion Disks in Active Galactic Nuclei","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Opacity; Active galactic nucleus; Thin disk; Accretion (finance); Thick disk; Accretion disc; Milky Way; Galaxy; Flux (metallurgy); Metallicity; Interstellar medium; Infrared; Astronomy; Optics; Halo","score_opus":0.015005299992363727,"score_gpt":0.28326085738203827,"score_spread":0.26825555738967455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062608889","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99712,0.0010506039,0.000074446514,0.000075540025,0.0000065011877,0.0000017648069,0.0000588921,0.000005855951,0.001606309],"genre_scores_gemma":[0.99855596,0.00042172216,0.00008328665,0.000053564978,0.000015187051,0.0000017753996,0.00007459576,0.000006743791,0.0007872318],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999138,0.000016877791,0.0000065426857,0.000019192428,0.000019115889,0.000024518498],"domain_scores_gemma":[0.9989354,0.0004219965,0.00031682578,0.00006657917,0.00006678355,0.000192325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020710737,0.00043891917,0.00017773312,0.0005291896,0.00039541454,0.0013206821,0.00040865078,0.00043160023,0.002845462],"category_scores_gemma":[0.0012451753,0.00025354262,0.00014139437,0.0002166306,0.0006210944,0.0006764183,0.00097527605,0.00048825674,0.0004315984],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023884997,0.00034589902,0.60750765,0.00041137155,0.00032160233,0.0032718957,0.00083491474,0.0089786025,0.33687976,0.0027040355,0.0010017678,0.035353974],"study_design_scores_gemma":[0.00006663986,0.0004947215,0.95139396,0.00012550951,0.00018350194,0.0014082945,0.0011116283,0.004287552,0.036925465,0.0019895688,0.0019812002,0.000031992942],"about_ca_topic_score_codex":0.0018318729,"about_ca_topic_score_gemma":0.0016104318,"teacher_disagreement_score":0.002845462,"about_ca_system_score_codex":0.00024910946,"about_ca_system_score_gemma":0.00010241737,"threshold_uncertainty_score":0.009519041},"labels":[],"label_agreement":null},{"id":"W2062717878","doi":"10.1088/0004-637x/799/1/60","title":"BRIGHTEST X-RAY CLUSTERS OF GALAXIES IN THE CFHTLS WIDE FIELDS: CATALOG AND OPTICAL MASS ESTIMATOR","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Luminosity; Galaxy; Estimator; Calibration; Sequence (biology); Spurious relationship; Galaxy cluster; Luminosity function","score_opus":0.010291066041107402,"score_gpt":0.21928764116290714,"score_spread":0.20899657512179973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062717878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96455705,0.00030877715,0.0030899954,0.00006098958,0.0000072397806,0.000078009754,0.027478332,0.000869975,0.0035496808],"genre_scores_gemma":[0.8617719,0.00020821698,0.012560529,0.00004243138,0.000048086833,0.00013015069,0.122604236,0.00010636062,0.002528094],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996101,0.000033392622,0.000029476474,0.000098658,0.00015801268,0.00007043176],"domain_scores_gemma":[0.9984363,0.00017918317,0.00037269146,0.00037716932,0.00036956495,0.00026517262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008801713,0.00027431993,0.00026655715,0.008495824,0.0003751173,0.00059705705,0.0005109785,0.00028144178,0.0043115425],"category_scores_gemma":[0.0018673491,0.00013870688,0.00024139085,0.003501002,0.00024864747,0.00042371952,0.0006354262,0.00014654233,0.0014367561],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017105551,0.00006500663,0.92935145,0.000072742485,0.000055334236,0.000099938065,0.00017735973,0.003813375,0.0068020714,0.0009036392,0.013282642,0.045205325],"study_design_scores_gemma":[0.000019825306,0.00002713232,0.9870112,0.000013345275,0.00001672725,0.000117631724,0.000050547536,0.006219218,0.0015064673,0.00015588831,0.004849649,0.00001237665],"about_ca_topic_score_codex":0.024467124,"about_ca_topic_score_gemma":0.024471523,"teacher_disagreement_score":0.024467124,"about_ca_system_score_codex":0.00069727085,"about_ca_system_score_gemma":0.0005897445,"threshold_uncertainty_score":0.04864937},"labels":[],"label_agreement":null},{"id":"W2062833044","doi":"10.1088/0004-637x/707/1/l69","title":"DIRECT EVIDENCE FOR OUTFLOW OF METAL-ENRICHED GAS ALONG THE RADIO JETS OF HYDRA A","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Outflow; Type-cD galaxy; Galaxy; X-shaped radio galaxy; Lernaean Hydra; Interacting galaxy; Metallicity; Radio galaxy; Galaxy cluster","score_opus":0.01898049252156853,"score_gpt":0.25304611233730057,"score_spread":0.23406561981573204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062833044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99892336,0.000070944254,0.00010184736,0.000028621538,0.0000042339984,0.0000027043686,0.00009249946,0.000029029623,0.0007466168],"genre_scores_gemma":[0.9992894,0.000050209477,0.00024977073,0.000034461245,0.000011411212,0.0000035574235,0.0001309858,0.0000072113335,0.00022303505],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999299,0.0000051293473,0.0000038464805,0.00002126826,0.000012293628,0.000027606588],"domain_scores_gemma":[0.9995029,0.00006873407,0.00016294033,0.000043762087,0.00004528709,0.00017636037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011003793,0.0002489079,0.00022504483,0.00053065445,0.0003946343,0.0007408868,0.00039112923,0.00030672667,0.0009686965],"category_scores_gemma":[0.0003874536,0.00032819918,0.00019001159,0.00023413761,0.0004897297,0.000296574,0.0009936648,0.00026271257,0.0002927157],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050876674,0.00011971514,0.70583534,0.00011006904,0.00013616154,0.001756209,0.00073060876,0.0004826481,0.2795071,0.0010046805,0.0006054687,0.0092032505],"study_design_scores_gemma":[0.000023149305,0.000094365474,0.9928703,0.000008879153,0.000036125115,0.0004772849,0.00018893003,0.0007263206,0.0045807534,0.00020461586,0.0007768295,0.000012485625],"about_ca_topic_score_codex":0.002619554,"about_ca_topic_score_gemma":0.0025042742,"teacher_disagreement_score":0.002619554,"about_ca_system_score_codex":0.00020425455,"about_ca_system_score_gemma":0.00014675278,"threshold_uncertainty_score":0.0052086115},"labels":[],"label_agreement":null},{"id":"W2062839084","doi":"10.1088/0004-637x/697/2/1164","title":"IMAGING THE BLACK HOLE SILHOUETTE OF M87: IMPLICATIONS FOR JET FORMATION AND BLACK HOLE SPIN","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":174,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Silhouette; Black hole (networking); Physics; Spin-flip; Spin (aerodynamics); Jet (fluid); Astrophysics; Carbon black; Galaxy; Materials science; Computer science; Artificial intelligence; Mechanics","score_opus":0.014941896759762936,"score_gpt":0.2609875143116664,"score_spread":0.24604561755190346,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2062839084","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9908635,0.00045794164,0.005463982,0.00029724327,0.0000084407675,0.000008816514,0.00014873373,0.000120774675,0.002630657],"genre_scores_gemma":[0.9983559,0.000098701814,0.0012886705,0.000033031785,0.00000805174,0.0000025533761,0.000072086565,0.000017684046,0.00012319797],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999324,0.000013085894,0.0000019859626,0.000013165783,0.000014947241,0.000024419942],"domain_scores_gemma":[0.9997049,0.00007961407,0.000098467324,0.000035920755,0.000021608752,0.00005955305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028226865,0.00035737874,0.00023775948,0.00047024895,0.00033765947,0.00090780435,0.00040058244,0.00045483178,0.00090970105],"category_scores_gemma":[0.0005586657,0.00024052979,0.00034260948,0.00027616264,0.0006892081,0.0005171322,0.00051340053,0.0003893701,0.00014874314],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065080886,0.00019396692,0.5467334,0.00025783462,0.00018231742,0.0016380739,0.0011485525,0.040950336,0.34191683,0.026603693,0.0025829105,0.037141234],"study_design_scores_gemma":[0.0000581092,0.00012775912,0.81751347,0.000047543996,0.00008152407,0.0005566645,0.00070327957,0.14960246,0.02008964,0.009342254,0.001829886,0.000047462814],"about_ca_topic_score_codex":0.0031789504,"about_ca_topic_score_gemma":0.0035178747,"teacher_disagreement_score":0.0031789504,"about_ca_system_score_codex":0.00054663845,"about_ca_system_score_gemma":0.00017552418,"threshold_uncertainty_score":0.0063208938},"labels":[],"label_agreement":null},{"id":"W2063101097","doi":"10.1086/376935","title":"Evidence of a Significant Intermediate-Age Population in the M31 Halo from Main-Sequence Photometry","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Andromeda Galaxy; Astronomy; Halo; Galaxy; Horizontal branch; Photometry (optics); Population; Galactic halo; Hubble space telescope; Advanced Camera for Surveys; Spiral galaxy; Stars","score_opus":0.022964798696383612,"score_gpt":0.252675181470272,"score_spread":0.2297103827738884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063101097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99891865,0.0001198773,0.00021320363,0.000008578376,6.320699e-7,0.0000026193497,0.000092057686,0.000010943475,0.00063352677],"genre_scores_gemma":[0.9995302,0.000037653594,0.00016468215,0.0000050354297,0.0000023696953,0.000001360219,0.00016663736,0.0000021780208,0.00008981373],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992883,0.000009109798,0.0000052058163,0.000018177469,0.000016658627,0.00002199738],"domain_scores_gemma":[0.9994949,0.00007402157,0.0001359625,0.00005660458,0.000053114007,0.0001853732],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020587606,0.0001822359,0.0001503145,0.0007594078,0.0002608469,0.00037303913,0.00016932645,0.0001720117,0.0017827053],"category_scores_gemma":[0.0005495703,0.000095126015,0.00014058061,0.00039802922,0.00024326857,0.00020372336,0.0005046781,0.00010262413,0.00040368875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022479462,0.000029097342,0.9563062,0.000026329057,0.000026170293,0.00018949364,0.0003224684,0.0005927576,0.03252276,0.00069330895,0.0001505445,0.008916082],"study_design_scores_gemma":[0.0000066403695,0.000086640495,0.9968382,0.000004364136,0.000012120935,0.00042064616,0.00008717475,0.0006555997,0.0010990885,0.00027867625,0.000506465,0.00000424875],"about_ca_topic_score_codex":0.0016102599,"about_ca_topic_score_gemma":0.0027581614,"teacher_disagreement_score":0.0017827053,"about_ca_system_score_codex":0.00013343604,"about_ca_system_score_gemma":0.000109770794,"threshold_uncertainty_score":0.0059638023},"labels":[],"label_agreement":null},{"id":"W2063128206","doi":"10.1088/0004-637x/723/2/1523","title":"THE ATACAMA COSMOLOGY TELESCOPE: PHYSICAL PROPERTIES AND PURITY OF A GALAXY CLUSTER SAMPLE SELECTED VIA THE SUNYAEV-ZEL'DOVICH EFFECT","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Redshift; ROSAT; Galaxy cluster; South Pole Telescope; Galaxy; Cosmology; Cluster (spacecraft); Telescope; Sky; Astronomy; Cluster sampling; Population","score_opus":0.005844130922634255,"score_gpt":0.2064595068739771,"score_spread":0.20061537595134285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063128206","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99436116,0.00006472621,0.00017182491,0.000059886057,0.0000049052614,0.000011934897,0.0038156214,0.000027387572,0.0014825144],"genre_scores_gemma":[0.9909719,0.000040617997,0.00046221793,0.00003262491,0.000013111494,0.000012386503,0.0073504755,0.000032576594,0.00108395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997533,0.000036497724,0.00001224801,0.000085436295,0.000064836044,0.00004767411],"domain_scores_gemma":[0.9988261,0.000115617586,0.00021837886,0.0001903416,0.00022342436,0.00042613986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050562783,0.00015063604,0.0003300898,0.0017316691,0.0011574064,0.0007781668,0.00048214514,0.0002745774,0.002785128],"category_scores_gemma":[0.0010978407,0.0001986678,0.00020174647,0.001852779,0.00039454718,0.0004230052,0.0008750015,0.00036422093,0.0009091794],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030425988,0.00012349486,0.9826836,0.000017426071,0.00010758917,0.00010678958,0.0006776249,0.0002082258,0.004892304,0.000499222,0.0045999703,0.005779477],"study_design_scores_gemma":[0.0000118875905,0.000010595964,0.99843234,0.0000014348478,0.000008519158,0.000042635493,0.00016261579,0.0002502176,0.0001821608,0.000038682767,0.0008554344,0.0000035160801],"about_ca_topic_score_codex":0.059788514,"about_ca_topic_score_gemma":0.07815962,"teacher_disagreement_score":0.059788514,"about_ca_system_score_codex":0.00056744524,"about_ca_system_score_gemma":0.00045922733,"threshold_uncertainty_score":0.11888105},"labels":[],"label_agreement":null},{"id":"W2063165454","doi":"10.1086/377249","title":"Relaxation of a Collisionless System and the Transition to a New Equilibrium Velocity Distribution","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Statistical Mechanics and Entropy","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Relaxation (psychology); Gaussian; Distribution (mathematics); Work (physics); Thermodynamic equilibrium; Numerical integration; Plasma; Velocity gradient","score_opus":0.007931380359274223,"score_gpt":0.2245866982732156,"score_spread":0.21665531791394138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063165454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9890248,0.00004089317,0.009880254,0.000051691248,0.0000058165465,0.000007175869,0.000010501593,0.000032184897,0.00094678625],"genre_scores_gemma":[0.99810493,0.00002203998,0.001557132,0.000011374102,0.000001949308,0.000004353348,0.000015860924,0.0000115336,0.00027096004],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999138,0.000015913054,0.000003825227,0.00001779304,0.000023471946,0.000025203368],"domain_scores_gemma":[0.9996668,0.000094796844,0.00007014088,0.000044402517,0.00005197501,0.00007183689],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030298004,0.0001293535,0.0002764126,0.00033427542,0.0007680759,0.00062467024,0.00045121452,0.0002606997,0.001107302],"category_scores_gemma":[0.0020634807,0.00015460819,0.00028038333,0.00015547319,0.0010025067,0.00067961484,0.0006097912,0.00040012828,0.00009344735],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054674776,0.00030968824,0.046990916,0.00009890663,0.00010655743,0.0013301419,0.0018682089,0.6940554,0.10956237,0.1251673,0.00054990017,0.019413916],"study_design_scores_gemma":[0.000051973635,0.00019345958,0.014195117,0.000007990843,0.000022355629,0.00028599246,0.0003013995,0.96167034,0.010648445,0.011715966,0.0008790482,0.000027905444],"about_ca_topic_score_codex":0.0039219963,"about_ca_topic_score_gemma":0.0024832664,"teacher_disagreement_score":0.0039219963,"about_ca_system_score_codex":0.00065242464,"about_ca_system_score_gemma":0.00051144336,"threshold_uncertainty_score":0.007798314},"labels":[],"label_agreement":null},{"id":"W2063210825","doi":"10.1088/0004-637x/750/2/167","title":"CUMULATIVE OXYGEN ABUNDANCES OF SPIRAL GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Abundance (ecology); Spiral (railway); Oxygen; Spiral galaxy; Galaxy; Chemical evolution; Astrophysics; Relative species abundance; Physics; Mathematics; Ecology; Biology; Mathematical analysis","score_opus":0.01813345747858691,"score_gpt":0.26646894946023997,"score_spread":0.24833549198165306,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063210825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948695,0.0005154548,0.0020057182,0.000023386474,0.000003768994,0.0000022415213,0.00031704624,0.0000667672,0.0021961792],"genre_scores_gemma":[0.9986676,0.00013515372,0.0005298612,0.000002972249,0.0000058355145,0.0000020477667,0.00026630063,0.000006782368,0.00038347914],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999248,0.0000042952256,0.000003819699,0.00003570438,0.000017244662,0.000014061614],"domain_scores_gemma":[0.99962974,0.00005879153,0.00010051569,0.000049357946,0.00009976238,0.00006188907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012246374,0.00020290006,0.00014924521,0.0012249314,0.000151198,0.00052105385,0.0002333805,0.00016332121,0.0006784326],"category_scores_gemma":[0.001092114,0.00011650589,0.00013819333,0.0004663888,0.0001947357,0.00033966298,0.00035722664,0.00010777287,0.00020929836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022518249,0.000016213276,0.84101725,0.00005511723,0.000089308356,0.00019368377,0.00038760126,0.012696788,0.09271128,0.005246003,0.00032045765,0.047041167],"study_design_scores_gemma":[0.000007765067,0.000077208686,0.9634158,0.0000113903025,0.00005115286,0.0003252731,0.0001931041,0.020180399,0.008818073,0.004513075,0.0023785115,0.000028325581],"about_ca_topic_score_codex":0.004709179,"about_ca_topic_score_gemma":0.003331529,"teacher_disagreement_score":0.004709179,"about_ca_system_score_codex":0.0004659187,"about_ca_system_score_gemma":0.00010095477,"threshold_uncertainty_score":0.009363532},"labels":[],"label_agreement":null},{"id":"W2063291404","doi":"10.1088/0004-637x/796/1/12","title":"LOWER LIMITS ON THE ANISOTROPY OF THE EXTRAGALACTIC GAMMA-RAY BACKGROUND IMPLIED BY THE 2FGL AND 1FHL CATALOGS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Anisotropy; Fermi Gamma-ray Space Telescope; Sky; Isotropy; Redshift; Point source; Population; Gamma ray; Astronomy; Galaxy; Optics","score_opus":0.009980357875754966,"score_gpt":0.21275829251921025,"score_spread":0.20277793464345528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063291404","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94601816,0.0016179576,0.013675227,0.00073607586,0.000034558303,0.000044488865,0.0122735305,0.00094589934,0.02465415],"genre_scores_gemma":[0.9802259,0.00020263328,0.005296398,0.0002630274,0.00008989637,0.000038478338,0.012917829,0.000114061586,0.0008518733],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9968315,0.0005445523,0.0001980104,0.0009589309,0.0007872229,0.0006798561],"domain_scores_gemma":[0.9821478,0.0056026718,0.00382159,0.00584577,0.0017215896,0.00086048903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0058392105,0.00057139195,0.0005166971,0.0069604893,0.0006133424,0.0036929601,0.0007954615,0.0008244782,0.0038939756],"category_scores_gemma":[0.013430088,0.00035473838,0.00065437285,0.0025826688,0.0007989937,0.0019658213,0.002022268,0.00047959108,0.0014522922],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005047783,0.000060579343,0.8930596,0.00016597373,0.00017467253,0.00032398387,0.0015336322,0.0026354403,0.008565673,0.02362382,0.0058516962,0.06350012],"study_design_scores_gemma":[0.00003320146,0.000030788262,0.974958,0.00009154698,0.00006146168,0.00028019494,0.00033967313,0.0038335558,0.002435335,0.005870615,0.012018445,0.000047106285],"about_ca_topic_score_codex":0.015059708,"about_ca_topic_score_gemma":0.017651292,"teacher_disagreement_score":0.015059708,"about_ca_system_score_codex":0.0012170654,"about_ca_system_score_gemma":0.00053519843,"threshold_uncertainty_score":0.030881107},"labels":[],"label_agreement":null},{"id":"W2063416986","doi":"10.1088/0004-637x/715/1/606","title":"THE ENVIRONMENTAL DEPENDENCE OF THE LUMINOSITY--SIZE RELATION FOR GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Fundamental plane (elliptical galaxies); Astrophysics; Luminosity; Galaxy; Luminosity function; Luminous infrared galaxy; Elliptical galaxy; Astronomy; Lenticular galaxy","score_opus":0.004621481587878746,"score_gpt":0.19301358380818498,"score_spread":0.18839210222030622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063416986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99702317,0.00019314453,0.00089950976,0.000029387378,0.0000015932275,0.000002482467,0.0006152652,0.000039591567,0.001195892],"genre_scores_gemma":[0.99821895,0.000060184993,0.00041148986,0.000009201657,0.000004267155,0.0000022861027,0.00096625555,0.000021654389,0.00030573033],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996357,0.00007639587,0.000020577243,0.00015016255,0.00005913885,0.00005801967],"domain_scores_gemma":[0.99594104,0.0014554113,0.0011690565,0.0006220346,0.0005341648,0.00027829432],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053933257,0.0002761163,0.00024399167,0.0014377191,0.00029239664,0.00068520824,0.00033392917,0.00019585276,0.001657811],"category_scores_gemma":[0.0034800938,0.00025461309,0.00026682872,0.0014888686,0.0003884012,0.0008079993,0.0007794459,0.00029747735,0.00053585024],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004605777,0.000019150197,0.9881544,0.000014434498,0.000059169135,0.000047580794,0.00012463951,0.0013633382,0.004331717,0.00033111035,0.00011381538,0.005394615],"study_design_scores_gemma":[0.0000013755568,0.000019633891,0.99723417,0.000001577684,0.000008714016,0.00006761659,0.000046828558,0.0011227312,0.0008213548,0.00017132671,0.0004983028,0.0000062825666],"about_ca_topic_score_codex":0.003662546,"about_ca_topic_score_gemma":0.007288733,"teacher_disagreement_score":0.003662546,"about_ca_system_score_codex":0.00031862894,"about_ca_system_score_gemma":0.000108940854,"threshold_uncertainty_score":0.0072824955},"labels":[],"label_agreement":null},{"id":"W2063433846","doi":"10.1088/0004-637x/779/2/103","title":"A NEW APPROACH TO DETAILED STRUCTURAL DECOMPOSITION FROM THE SPLASH AND PHAT SURVEYS: KICKED-UP DISK STARS IN THE ANDROMEDA GALAXY?","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Bulge; Andromeda Galaxy; Andromeda; Halo; Stars; Galaxy; Astronomy; Population; Thick disk; Spiral galaxy; Milky Way","score_opus":0.009088094864138198,"score_gpt":0.220419896969706,"score_spread":0.2113318021055678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063433846","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.32610753,0.00032011635,0.66673595,0.0004534534,0.000023364197,0.00013359239,0.0020536734,0.00095638883,0.0032158724],"genre_scores_gemma":[0.8171564,0.00024577059,0.17777894,0.000116049196,0.00004843998,0.0001217673,0.003084136,0.00017771797,0.0012707158],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.999762,0.00006499428,0.000014961749,0.0000796329,0.000047179128,0.000031214353],"domain_scores_gemma":[0.99895906,0.0002750355,0.00027845163,0.0002713021,0.00011210376,0.00010409633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006782577,0.00044379025,0.00054957136,0.0017273369,0.0003720096,0.0012491376,0.0007551818,0.00057141803,0.0013204927],"category_scores_gemma":[0.00326085,0.00043487235,0.0008492226,0.0010403497,0.00046780004,0.0009756999,0.0011635083,0.00065970013,0.00045261474],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031432995,0.0001835484,0.23320305,0.00023463865,0.00036557636,0.00042719854,0.0013078254,0.41385671,0.025726499,0.06933807,0.0032348312,0.25180775],"study_design_scores_gemma":[0.000015114116,0.000052519972,0.032734923,0.00003455573,0.000024463427,0.00018458297,0.00018124981,0.92728347,0.0014870487,0.034841172,0.0031177073,0.00004310923],"about_ca_topic_score_codex":0.009432885,"about_ca_topic_score_gemma":0.011587053,"teacher_disagreement_score":0.009432885,"about_ca_system_score_codex":0.00065842224,"about_ca_system_score_gemma":0.0006556023,"threshold_uncertainty_score":0.018755972},"labels":[],"label_agreement":null},{"id":"W2063511228","doi":"10.1086/374735","title":"High‐Resolution Spectroscopy of the Pulsating White Dwarf G29‐38","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Spectral line; Light curve; Flux (metallurgy); Fourier transform; Amplitude; Doppler effect; Harmonic; Fourier analysis; White dwarf","score_opus":0.008503897737299641,"score_gpt":0.21817090123343122,"score_spread":0.20966700349613157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063511228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99870694,0.00008074664,0.00039677593,0.000021780947,0.000002626854,0.0000031692223,0.000120734556,0.000024326318,0.000642953],"genre_scores_gemma":[0.99821484,0.000046931862,0.0010417077,0.00001287203,0.000006098743,0.0000033003673,0.00028461477,0.0000075900157,0.00038210195],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999645,0.0000025938782,0.0000010797467,0.000011948794,0.000012562622,0.000007342606],"domain_scores_gemma":[0.9999007,0.000018454311,0.000018903353,0.000012437182,0.000018625837,0.0000308825],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000114768765,0.00017437832,0.00013400396,0.0003675179,0.00022148754,0.00016344522,0.00018732762,0.00020168549,0.00061025604],"category_scores_gemma":[0.0001755056,0.00007659998,0.00011114002,0.00023882958,0.00012195507,0.00014682444,0.00017596036,0.00020361131,0.00015885918],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023556406,0.000085043925,0.052451227,0.000052568263,0.000044333457,0.00066565827,0.00030913472,0.00084942114,0.9310652,0.00020095418,0.00039851342,0.013642494],"study_design_scores_gemma":[0.00003765283,0.00037803643,0.91292834,0.000013060832,0.000044149856,0.0018896207,0.00023968781,0.004212345,0.0762715,0.00040590277,0.0035582548,0.000021490569],"about_ca_topic_score_codex":0.0009197662,"about_ca_topic_score_gemma":0.0013571655,"teacher_disagreement_score":0.0009197662,"about_ca_system_score_codex":0.00010498934,"about_ca_system_score_gemma":0.000057413818,"threshold_uncertainty_score":0.0020415187},"labels":[],"label_agreement":null},{"id":"W2063728816","doi":"10.1088/0004-637x/696/2/1918","title":"FAR-INFRARED OBSERVATIONS OF THE VERY LOW LUMINOSITY EMBEDDED SOURCE L1521F-IRS IN THE TAURUS STAR-FORMING REGION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Astrophysics; Physics; Extinction (optical mineralogy); Luminosity; Opacity; Interstellar medium; Infrared; Star formation; Molecular cloud; Astronomy; Young stellar object; Stars; Galaxy","score_opus":0.018361661087711312,"score_gpt":0.2322966471971733,"score_spread":0.213934986109462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063728816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864715,0.00007515105,0.00010941236,0.000014268844,0.0000021116791,0.000002735323,0.00024781586,0.000019953899,0.00088126416],"genre_scores_gemma":[0.9981775,0.00005860655,0.00037225155,0.000020507918,0.000009987129,0.000004971457,0.0010912218,0.0000090380945,0.0002558662],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998412,0.000011380053,0.000008938663,0.000054772452,0.00003810948,0.00004557664],"domain_scores_gemma":[0.9994475,0.00003693236,0.00023595551,0.000062381194,0.000053006595,0.00016418807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031159044,0.00034050384,0.00029234504,0.00089443114,0.00041311144,0.00064445444,0.00058891374,0.00033844617,0.0007324964],"category_scores_gemma":[0.00046872802,0.00019588489,0.0003351814,0.00065774395,0.00027251214,0.00036604688,0.0005104498,0.00027519488,0.00056788535],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024317761,0.00024012342,0.8545478,0.000048900107,0.00012390933,0.0006516185,0.0005297561,0.0014986554,0.12724392,0.000363168,0.00063547486,0.013873456],"study_design_scores_gemma":[0.0000064609817,0.00005026535,0.99740064,0.000003564318,0.000015193658,0.00014385224,0.000057639292,0.0006131448,0.0012206476,0.000039809758,0.0004436932,0.0000050343137],"about_ca_topic_score_codex":0.0051815263,"about_ca_topic_score_gemma":0.009020787,"teacher_disagreement_score":0.0051815263,"about_ca_system_score_codex":0.00055262534,"about_ca_system_score_gemma":0.00016662941,"threshold_uncertainty_score":0.010302722},"labels":[],"label_agreement":null},{"id":"W2063754867","doi":"10.1086/523668","title":"The Mid‐Infrared Spectral Energy Distribution, Surface Brightness, and Color Profiles in Elliptical Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Surface brightness; Elliptical galaxy; Galaxy; Surface brightness fluctuation; RADIUS; Brightness; Metallicity; Spectral energy distribution; Emission spectrum","score_opus":0.0059632135559157156,"score_gpt":0.19223796496897855,"score_spread":0.18627475141306282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063754867","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996,0.000023030316,0.000054589567,0.000005164936,2.2881993e-7,7.6533354e-7,0.0001249923,0.0000043979703,0.00018682855],"genre_scores_gemma":[0.9990804,0.00002942797,0.00016315455,0.00000529275,0.000001737457,0.0000025392446,0.0005007318,0.0000035558114,0.00021311738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998896,0.000012010733,0.000007743686,0.000036453825,0.000022574075,0.00003165044],"domain_scores_gemma":[0.9995778,0.00005193144,0.0001661822,0.00004946796,0.000067360845,0.000087210654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002137369,0.00013395336,0.0001432846,0.001556642,0.0001933641,0.0004535407,0.000176524,0.00018701529,0.00080540875],"category_scores_gemma":[0.00055490766,0.00015302215,0.0001733399,0.00066515215,0.00019068786,0.00030909243,0.0003111434,0.00011592443,0.00043624957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055259436,0.000022312866,0.990659,0.0000030293347,0.000014717977,0.000035473826,0.00021166164,0.00010987807,0.004826118,0.000037451362,0.0000685735,0.003956559],"study_design_scores_gemma":[3.7912287e-7,0.0000057921447,0.9996594,5.256657e-7,0.0000015113374,0.00003485823,0.000041520063,0.00008519396,0.00009123501,0.000009442347,0.00006940125,8.292731e-7],"about_ca_topic_score_codex":0.004348602,"about_ca_topic_score_gemma":0.006024464,"teacher_disagreement_score":0.004348602,"about_ca_system_score_codex":0.00023549165,"about_ca_system_score_gemma":0.000061791274,"threshold_uncertainty_score":0.008646607},"labels":[],"label_agreement":null},{"id":"W2063756557","doi":"10.1088/0004-637x/716/2/907","title":"ON POSSIBLE VARIATION IN THE COSMOLOGICAL BARYON FRACTION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Baryon; Dark matter; Big Bang nucleosynthesis; Galaxy; Galaxy cluster; Anisotropy; Astronomy; Nucleosynthesis; Stars","score_opus":0.007227575937494957,"score_gpt":0.25259316443575697,"score_spread":0.245365588498262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063756557","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9821354,0.00029542853,0.008071619,0.00018648141,0.000012805567,0.00000598352,0.00065546745,0.000058529196,0.008578329],"genre_scores_gemma":[0.9988839,0.00006918458,0.00059445814,0.000017436141,0.0000052221144,0.0000023918024,0.00019269343,0.0000120185,0.00022282975],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997435,0.000076533615,0.000009289595,0.000092069226,0.000043598604,0.000034972276],"domain_scores_gemma":[0.99776983,0.0014968729,0.000271059,0.00027169177,0.000114437404,0.00007609832],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067669584,0.00029622982,0.0002307781,0.00058723334,0.0002537276,0.0006229283,0.00037630502,0.000268204,0.0030514507],"category_scores_gemma":[0.0046034805,0.0001318721,0.00021408097,0.00062320475,0.00043002734,0.0005834213,0.00034684682,0.00022504975,0.00025628434],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011740881,0.000111783535,0.70357275,0.00020260658,0.0005342154,0.0012018413,0.00062977325,0.09362226,0.053209934,0.07939938,0.0014203459,0.06492101],"study_design_scores_gemma":[0.000028430202,0.00012913396,0.8016093,0.000056176716,0.00013043528,0.00046924004,0.00024198834,0.13067783,0.020110408,0.042008147,0.004461116,0.00007785743],"about_ca_topic_score_codex":0.002135663,"about_ca_topic_score_gemma":0.0025342323,"teacher_disagreement_score":0.0030514507,"about_ca_system_score_codex":0.00033539874,"about_ca_system_score_gemma":0.00014764631,"threshold_uncertainty_score":0.01020813},"labels":[],"label_agreement":null},{"id":"W2063790219","doi":"10.1086/498058","title":"Globular Cluster Systems in Brightest Cluster Galaxies: Bimodal Metallicity Distributions and the Nature of the High‐Luminosity Clusters","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":222,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Astrophysics; Globular cluster; Physics; Astronomy; Metallicity; Galaxy; Elliptical galaxy; Galaxy cluster; Photometry (optics); Brightest cluster galaxy; Population; Stars","score_opus":0.003746547136840624,"score_gpt":0.19537563455771126,"score_spread":0.19162908742087065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063790219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999466,0.00009370756,0.000071739356,0.000018452482,5.275204e-7,6.4069957e-7,0.00004054561,0.0000051382654,0.00030332862],"genre_scores_gemma":[0.9998386,0.000016963493,0.000038331356,0.000007652714,0.0000019506595,5.043826e-7,0.000039334478,0.0000014696222,0.00005523001],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998627,0.0000124215485,0.000007051202,0.000042659205,0.000020155665,0.000054995035],"domain_scores_gemma":[0.9984675,0.00021590784,0.0006230639,0.0001270995,0.00014998164,0.00041636184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026887783,0.00010542827,0.00017534253,0.0012379675,0.0003451245,0.0007557703,0.00023221056,0.0003187745,0.0019472083],"category_scores_gemma":[0.001198307,0.00013307644,0.0000785587,0.0005296241,0.0006487886,0.00048596002,0.00066663016,0.00020129127,0.00025128358],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016221171,0.000016514583,0.980735,0.000015344389,0.000015221014,0.00008250144,0.00059124955,0.00021099231,0.012792359,0.00045412598,0.00011810778,0.0048063756],"study_design_scores_gemma":[0.0000035982996,0.000013628208,0.99885476,0.0000022764857,0.0000050960844,0.00015146729,0.000094151204,0.00015601878,0.00036596545,0.00023576521,0.00011413403,0.0000030618774],"about_ca_topic_score_codex":0.003167174,"about_ca_topic_score_gemma":0.0057560755,"teacher_disagreement_score":0.003167174,"about_ca_system_score_codex":0.00035243775,"about_ca_system_score_gemma":0.00012710156,"threshold_uncertainty_score":0.006514013},"labels":[],"label_agreement":null},{"id":"W2063812950","doi":"10.1088/0004-637x/757/2/180","title":"THE INTRINSIC FRACTIONS AND RADIO PROPERTIES OF LOW-IONIZATION BROAD ABSORPTION LINE QUASARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Quasar; Population; Absorption (acoustics); Line (geometry); Fraction (chemistry); Spectral line","score_opus":0.009846946075969792,"score_gpt":0.21015939898350802,"score_spread":0.20031245290753824,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063812950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99783957,0.00035308898,0.0002945283,0.00003005842,0.000002931093,0.0000023774503,0.0002107882,0.000012653794,0.0012539383],"genre_scores_gemma":[0.99847764,0.00022015547,0.00007819715,0.000028346203,0.000027903037,0.0000024211859,0.0003432155,0.000007280934,0.00081494014],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999931,0.0000101977175,0.000004579394,0.000017882383,0.000011217351,0.000025231097],"domain_scores_gemma":[0.99891436,0.00038714823,0.0002929025,0.00007746547,0.000102650425,0.00022547081],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004842027,0.0002900303,0.00021989111,0.0010910097,0.00023866774,0.0008546591,0.00038361896,0.00030513213,0.005670389],"category_scores_gemma":[0.0014274829,0.0001984985,0.00017934506,0.00042066764,0.0003228924,0.00070380303,0.00033279334,0.0003069361,0.0008272238],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044491063,0.0000947818,0.95379275,0.000041381005,0.00006716365,0.00015697541,0.00020201689,0.000292649,0.033826534,0.0005769045,0.00020902995,0.010294914],"study_design_scores_gemma":[0.0000040434775,0.000051693958,0.99819547,0.000002021462,0.000015587633,0.00013166104,0.00006293318,0.0001278678,0.0010929843,0.00015690792,0.00015607975,0.000002714789],"about_ca_topic_score_codex":0.0005669322,"about_ca_topic_score_gemma":0.0005598123,"teacher_disagreement_score":0.005670389,"about_ca_system_score_codex":0.00019105093,"about_ca_system_score_gemma":0.00006042769,"threshold_uncertainty_score":0.018969357},"labels":[],"label_agreement":null},{"id":"W2063956712","doi":"10.1086/320911","title":"The Evolutionary Timescale of Sakurai’s Object: A Test of Convection Theory?","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Stellar evolution; Astrophysics; Convection; White dwarf; Mixing (physics); Asymptotic giant branch; Stellar mass; Convection zone; Thermal; Stars; Astronomy; Star formation; Mechanics","score_opus":0.006275294391865492,"score_gpt":0.21105390209417918,"score_spread":0.20477860770231368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2063956712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98067814,0.0032126058,0.0022477643,0.0023188242,0.00015925018,0.000014686752,0.00027788192,0.0000839352,0.011006943],"genre_scores_gemma":[0.99899596,0.00023526754,0.0002906211,0.00008650841,0.00006378791,0.000005864831,0.00008679806,0.000024987592,0.0002101941],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980825,0.000028710563,0.00001275677,0.00008285712,0.000019463441,0.00004797406],"domain_scores_gemma":[0.99853456,0.0004873237,0.0004014978,0.00014662772,0.00010405408,0.00032597056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012634221,0.00031141643,0.00044863432,0.00045170853,0.00064470386,0.0012696668,0.0007005376,0.00064945646,0.0030193655],"category_scores_gemma":[0.0038049314,0.00016186389,0.0004872597,0.00031819972,0.0006589756,0.0021767963,0.0010457833,0.00065249775,0.00056796573],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002371299,0.00015433464,0.7720109,0.000780202,0.00039200688,0.0012363539,0.003376822,0.0064378665,0.057244003,0.07434991,0.0032122082,0.07843414],"study_design_scores_gemma":[0.00023216961,0.0004313331,0.90809935,0.00012034881,0.0002139516,0.00084289355,0.0014575447,0.036270395,0.003776108,0.040804088,0.0076707075,0.000081129765],"about_ca_topic_score_codex":0.0023412448,"about_ca_topic_score_gemma":0.0006463656,"teacher_disagreement_score":0.0030193655,"about_ca_system_score_codex":0.0007450769,"about_ca_system_score_gemma":0.00031614894,"threshold_uncertainty_score":0.010100782},"labels":[],"label_agreement":null},{"id":"W2064000743","doi":"10.1086/524098","title":"<i>XMM‐Newton</i>,<i>Chandra</i>, and CGPS observations of the Supernova Remnants G85.4+0.7 and G85.9−0.6","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University; University of Calgary; Herzberg Institute of Astrophysics; Research Canada; University of Manitoba","funders":"","keywords":"Supernova; Near-Earth supernova; Pulsar; Computational astrophysics; Gamma-ray astronomy; Shock wave","score_opus":0.01898175064423786,"score_gpt":0.2071995655354394,"score_spread":0.18821781489120154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064000743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.80653954,0.0043945736,0.0017249952,0.011591539,0.0029650673,0.00042544547,0.03842081,0.0025681746,0.1313699],"genre_scores_gemma":[0.7614037,0.002978037,0.0055360864,0.0022274465,0.004354247,0.00012069411,0.058203604,0.00071459846,0.16446167],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9995672,0.000020541054,0.000027440503,0.00006117648,0.0002629297,0.00006069223],"domain_scores_gemma":[0.9976599,0.00011732815,0.0006196179,0.00024445288,0.0009943319,0.0003642841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006452171,0.00028167776,0.00034721653,0.0027190517,0.0006792885,0.00094508985,0.0004572706,0.00064407743,0.022555046],"category_scores_gemma":[0.0023272133,0.00023061136,0.0002473095,0.0012253532,0.0002643258,0.0006985638,0.00070554507,0.0004214495,0.0063248416],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014832735,0.00023276555,0.3621475,0.001009029,0.00024803242,0.0023146805,0.0006843494,0.00042280566,0.048712,0.0028748948,0.38296583,0.19690488],"study_design_scores_gemma":[0.000054366777,0.00007195768,0.8822548,0.000062850115,0.000057579266,0.00043429076,0.00014570757,0.00019398138,0.004726904,0.00034261946,0.11163276,0.00002222802],"about_ca_topic_score_codex":0.005422734,"about_ca_topic_score_gemma":0.017429749,"teacher_disagreement_score":0.022555046,"about_ca_system_score_codex":0.0003495522,"about_ca_system_score_gemma":0.00052080164,"threshold_uncertainty_score":0.075454175},"labels":[],"label_agreement":null},{"id":"W2064203322","doi":"10.1088/0004-637x/783/2/99","title":"ON THE X-RAY VARIABILITY OF MAGNETAR 1RXS J170849.0–400910","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Glitch; Magnetar; Pulsar; Flux (metallurgy); Neutron star; QUIET; Spectral line; Spectral analysis","score_opus":0.009434833662676105,"score_gpt":0.21010380304138596,"score_spread":0.20066896937870984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064203322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988675,0.0000925339,0.00006993311,0.000029074907,0.0000046126893,0.000003132355,0.0004269726,0.000012351002,0.00049397297],"genre_scores_gemma":[0.9970561,0.00010222522,0.00026116826,0.000026964768,0.000030862233,0.0000064023548,0.0022210684,0.000011496939,0.000283622],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998926,0.000008163043,0.000008004882,0.00003315274,0.000027851776,0.00003025139],"domain_scores_gemma":[0.99950993,0.00005185126,0.00023863933,0.000036589652,0.00008188361,0.00008113389],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027432333,0.00026274988,0.00022960192,0.0014670576,0.00036116596,0.00036284784,0.00025415275,0.0002801295,0.0006196508],"category_scores_gemma":[0.00051101943,0.000105240935,0.00023205871,0.0010861787,0.00022946601,0.00026431167,0.00046231574,0.0002465909,0.0002557949],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033580535,0.00012279495,0.93659234,0.00007708591,0.00014752,0.0015623675,0.00046986787,0.0023349281,0.041315697,0.00028906047,0.0014358833,0.015316571],"study_design_scores_gemma":[0.0000021460028,0.000022810915,0.9985012,0.0000033671652,0.000011419993,0.00020138157,0.000045671866,0.00035629724,0.00031989836,0.000024772067,0.00050728256,0.0000036579174],"about_ca_topic_score_codex":0.0036119574,"about_ca_topic_score_gemma":0.009941388,"teacher_disagreement_score":0.0036119574,"about_ca_system_score_codex":0.00030736072,"about_ca_system_score_gemma":0.00014148743,"threshold_uncertainty_score":0.007181883},"labels":[],"label_agreement":null},{"id":"W2064278103","doi":"10.1088/0004-637x/742/1/17","title":"CONSTRAINTS ON THE MASS AND RADIUS OF THE NEUTRON STAR XTE J1807-294","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Calgary","funders":"","keywords":"Physics; Schwarzschild radius; RADIUS; Millisecond pulsar; Neutron star; Astrophysics; Black-body radiation; Light curve; Solar mass; Accretion (finance); Pulsar; Solar radius; Astronomy; Radiation; Nuclear physics; Stars; Coronal mass ejection; Plasma","score_opus":0.021016679831310607,"score_gpt":0.27524791095302875,"score_spread":0.25423123112171814,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064278103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99482757,0.00015839381,0.0026060364,0.000044322966,0.0000034784364,0.0000028442475,0.00010700967,0.000035593686,0.0022148467],"genre_scores_gemma":[0.998872,0.000061954735,0.00072807656,0.000007143078,0.0000055804744,0.0000031917925,0.00020551044,0.000011706689,0.00010488772],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99989223,0.000021315054,0.0000073568644,0.00002796136,0.000033510303,0.000017582228],"domain_scores_gemma":[0.9990711,0.00046975125,0.00023852775,0.00009535438,0.00005956981,0.00006558756],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037533426,0.0004202392,0.00036761828,0.0005894773,0.00045327403,0.0006564901,0.00059336534,0.00048841734,0.00068028946],"category_scores_gemma":[0.002007433,0.00030343418,0.0003277177,0.00022099371,0.00036893805,0.0004738593,0.0007073791,0.00030183402,0.00030883588],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011443357,0.00011530936,0.5948085,0.00018308971,0.00021744719,0.0019495216,0.0004954726,0.12248734,0.22829412,0.021874748,0.0010909679,0.027339187],"study_design_scores_gemma":[0.000143771,0.00047524567,0.4329403,0.000080606704,0.00013216064,0.002442794,0.0003074049,0.49401036,0.046227682,0.01668847,0.0064457543,0.00010551868],"about_ca_topic_score_codex":0.0009797342,"about_ca_topic_score_gemma":0.0010277061,"teacher_disagreement_score":0.0009797342,"about_ca_system_score_codex":0.0002855144,"about_ca_system_score_gemma":0.00016687014,"threshold_uncertainty_score":0.0022758245},"labels":[],"label_agreement":null},{"id":"W2064302459","doi":"10.1086/317304","title":"Discovery of a Disk-collimated Bipolar Outflow in the Proto–Planetary Nebula IRAS 17106−3046","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Planetary nebula; Collimated light; Bipolar outflow; Astronomy; Bipolar nebula; Astrophysics; Outflow; Nebula; Emission nebula; Stars; Optics; Star formation","score_opus":0.008172710576477006,"score_gpt":0.22497010457163302,"score_spread":0.21679739399515602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064302459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963419,0.0005509927,0.00038283644,0.000086284505,0.000034090157,0.000019922787,0.0001935975,0.000025810881,0.0023645803],"genre_scores_gemma":[0.9969452,0.00018799628,0.001535793,0.00016744192,0.00004541278,0.000011886524,0.00054752786,0.000006578074,0.0005521417],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999136,0.0000061944356,0.000005399952,0.000019756177,0.000030949002,0.000024163313],"domain_scores_gemma":[0.99967957,0.000025845486,0.00011358757,0.00003406828,0.00004373561,0.00010325828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000205784,0.00024949166,0.00027664253,0.00063264044,0.0008071662,0.00072816043,0.00039108077,0.0008817985,0.00092645193],"category_scores_gemma":[0.00032304696,0.00018465018,0.00016856498,0.00052397745,0.0003944735,0.00025332562,0.00066175323,0.00052033894,0.00073573267],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076752185,0.00027042636,0.31216025,0.00025980792,0.00009195249,0.031077662,0.001021481,0.0005612761,0.6194885,0.0015815123,0.0020795271,0.030640136],"study_design_scores_gemma":[0.000069317255,0.0009284591,0.91908526,0.00003741954,0.000054337062,0.039585136,0.0005493287,0.00091404637,0.022082627,0.00078438537,0.015857251,0.00005233793],"about_ca_topic_score_codex":0.0007809783,"about_ca_topic_score_gemma":0.0011949064,"teacher_disagreement_score":0.00092645193,"about_ca_system_score_codex":0.0002579877,"about_ca_system_score_gemma":0.0002152505,"threshold_uncertainty_score":0.0030993223},"labels":[],"label_agreement":null},{"id":"W2064307980","doi":"10.1088/0004-637x/738/1/3","title":"VERITAS OBSERVATIONS OF THE TeV BINARY LS I +61° 303 DURING 2008-2010","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Crab Nebula; Telescope; MAGIC (telescope); Flux (metallurgy); Astronomy; Proportional counter; Light curve; Nebula; Binary number; Gamma ray; Stars","score_opus":0.023525106643140607,"score_gpt":0.2066287466418169,"score_spread":0.1831036399986763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064307980","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99698466,0.00007918473,0.00010141576,0.000021087882,0.0000052789187,0.0000073584956,0.00095886877,0.000026946871,0.0018153458],"genre_scores_gemma":[0.99402964,0.000086293454,0.00057978486,0.00003477936,0.000015413128,0.000012189985,0.0041593006,0.000017857352,0.0010647941],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998098,0.000012002733,0.000009823148,0.000046411245,0.00007806958,0.000043949203],"domain_scores_gemma":[0.9995473,0.00004685462,0.00019752528,0.000040208724,0.00008643845,0.00008168217],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029449994,0.0001877217,0.0003031404,0.0009765965,0.0005904329,0.0005205433,0.00024703355,0.00028941047,0.0012620793],"category_scores_gemma":[0.00040208927,0.00021741877,0.00018176908,0.0007105153,0.00025419978,0.0002813723,0.00075768563,0.00043679215,0.00042289754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017627748,0.00021847461,0.82616884,0.0001554118,0.00011133558,0.001079627,0.0015530788,0.0012393387,0.12931314,0.0005322605,0.003257304,0.034608494],"study_design_scores_gemma":[0.00002225943,0.00018751678,0.9949706,0.000013784351,0.000020418553,0.00035571266,0.00014188838,0.00038971944,0.001945462,0.000027712931,0.0019162003,0.000008754517],"about_ca_topic_score_codex":0.013151177,"about_ca_topic_score_gemma":0.06748415,"teacher_disagreement_score":0.013151177,"about_ca_system_score_codex":0.0007744284,"about_ca_system_score_gemma":0.00044246053,"threshold_uncertainty_score":0.026149213},"labels":[],"label_agreement":null},{"id":"W2064377545","doi":"10.1086/589503","title":"Shell Revealed in SN 1979C","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Shell (structure); Luminosity; Supernova; Galaxy; Very-long-baseline interferometry; Brightness; Surface brightness; Crab Nebula; Ridge; Flux (metallurgy)","score_opus":0.013989184518751674,"score_gpt":0.22504084208855377,"score_spread":0.2110516575698021,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064377545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905235,0.00034060946,0.00020238824,0.00004989402,0.000027913746,0.000014586704,0.000827717,0.00005573692,0.007957577],"genre_scores_gemma":[0.9943402,0.000233656,0.0005903212,0.00013265385,0.000022172277,0.000011690421,0.0023777764,0.000028239352,0.0022632985],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998592,0.000005967132,0.000008754402,0.000036843074,0.00004260568,0.000046693553],"domain_scores_gemma":[0.9996753,0.00001972581,0.00008878652,0.000040482228,0.00006652276,0.00010920366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013856318,0.00021094136,0.00032588447,0.0010381413,0.0005986562,0.0005420294,0.00021979216,0.00043801573,0.0021223358],"category_scores_gemma":[0.00045445323,0.00015841627,0.00023347865,0.0005108889,0.0002779271,0.00012397887,0.0005866991,0.00030677317,0.0007292632],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011978946,0.00020129787,0.7866508,0.00008430238,0.00011949525,0.009564593,0.00039886526,0.00033258047,0.16377054,0.0028346416,0.0038481278,0.03099698],"study_design_scores_gemma":[0.000022527087,0.000094920215,0.97010744,0.00001866352,0.000043612214,0.010048725,0.0001242759,0.00033185715,0.009110038,0.00029532347,0.009785722,0.000016974882],"about_ca_topic_score_codex":0.023408554,"about_ca_topic_score_gemma":0.026937785,"teacher_disagreement_score":0.023408554,"about_ca_system_score_codex":0.0007076959,"about_ca_system_score_gemma":0.0004019701,"threshold_uncertainty_score":0.04654461},"labels":[],"label_agreement":null},{"id":"W2064417845","doi":"10.1086/507830","title":"Ejection of High‐Velocity Stars from the Galactic Center by an Inspiraling Intermediate‐Mass Black Hole","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Stars; Galactic Center; Black hole (networking); Stellar dynamics; Galaxy; Neutron star; Cusp (singularity); Stellar collision; Orbit (dynamics)","score_opus":0.009920119603114739,"score_gpt":0.21927876829586992,"score_spread":0.2093586486927552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064417845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99438596,0.00009642376,0.00457841,0.00003692511,0.0000041134895,0.0000037168804,0.000028412733,0.000035844652,0.000830147],"genre_scores_gemma":[0.99865997,0.000060421426,0.0008378163,0.000009429955,0.0000041897883,0.0000010808069,0.00004667047,0.000008405473,0.00037199561],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999664,0.0000045139,0.000001692427,0.0000071176746,0.000007087073,0.000013238489],"domain_scores_gemma":[0.9998036,0.000041610885,0.00006721247,0.000023733011,0.000018525341,0.00004540893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024120335,0.00028474073,0.00024007088,0.0004931201,0.00033164932,0.0006102017,0.0004594502,0.00033758898,0.00065931893],"category_scores_gemma":[0.00090893556,0.00019988306,0.00040719446,0.00021959255,0.0003400753,0.000522344,0.00048468617,0.0002389403,0.00012519871],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040207445,0.000152006,0.723818,0.00010292903,0.00015850803,0.0035327997,0.0006477408,0.118982345,0.07808248,0.040676065,0.00085822184,0.032586843],"study_design_scores_gemma":[0.00009037659,0.0002232352,0.41165376,0.00002855795,0.00006917047,0.0019806328,0.00035317318,0.5551219,0.0154861435,0.013443112,0.0015045581,0.000045391494],"about_ca_topic_score_codex":0.005668664,"about_ca_topic_score_gemma":0.0054619783,"teacher_disagreement_score":0.005668664,"about_ca_system_score_codex":0.00066383235,"about_ca_system_score_gemma":0.00019560773,"threshold_uncertainty_score":0.011271358},"labels":[],"label_agreement":null},{"id":"W2064745170","doi":"10.1088/0004-637x/725/2/2110","title":"INFLUENCE OF TURBULENCE DISSIPATION EFFECTS ON THE PROPAGATION OF LOW-ENERGY COSMIC RAYS IN THE GALAXY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Cosmic ray; Dissipation; Diffusion; Particle acceleration; Galaxy; Computational physics; Turbulence; Scattering; Astrophysics; Particle (ecology); Acceleration; Range (aeronautics); Mechanics; Classical mechanics; Optics; Quantum mechanics","score_opus":0.003144153017645609,"score_gpt":0.20609782729428847,"score_spread":0.20295367427664285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064745170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996345,0.00012255929,0.0022490812,0.00007778241,0.000012395106,0.000005239171,0.000023554372,0.00006481929,0.0010996158],"genre_scores_gemma":[0.99976295,0.000022622873,0.00014938517,0.0000032411253,0.0000024253804,7.945204e-7,0.000009342905,0.0000071831837,0.000042083735],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984574,0.00004946645,0.000011586531,0.000021123202,0.000027563909,0.000044571825],"domain_scores_gemma":[0.9990243,0.0004659127,0.00018921912,0.000070227135,0.00010595794,0.00014441699],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003639346,0.00057796447,0.00030261488,0.0006044651,0.00038643714,0.001024586,0.00021448018,0.0002768684,0.00035113387],"category_scores_gemma":[0.0027173802,0.00023544901,0.00042861458,0.00027762938,0.0006810812,0.0004965942,0.0005085056,0.00037264713,0.00006663113],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013944672,0.00021270022,0.21807995,0.00011695577,0.00027213682,0.0016115528,0.0003225567,0.56006193,0.18982916,0.0132661555,0.00045548906,0.014376903],"study_design_scores_gemma":[0.00010507673,0.0001670823,0.09524093,0.000014651445,0.000080136626,0.00014470321,0.00006304427,0.882999,0.019245308,0.0016671042,0.00020180726,0.000071138755],"about_ca_topic_score_codex":0.010972175,"about_ca_topic_score_gemma":0.0036135882,"teacher_disagreement_score":0.010972175,"about_ca_system_score_codex":0.00080127874,"about_ca_system_score_gemma":0.0003590334,"threshold_uncertainty_score":0.021816611},"labels":[],"label_agreement":null},{"id":"W2064760621","doi":"10.1086/520123","title":"<i>Spitzer</i>Observations of Transient, Extended Dust in Two Elliptical Galaxies: New Evidence of Recent Feedback Energy Release in Galactic Cores","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Galaxy; Dust lane; Outflow; Elliptical galaxy; Hubble sequence; Interstellar medium; Star formation; Cooling flow; Active galactic nucleus","score_opus":0.02647647871197221,"score_gpt":0.2682152005092382,"score_spread":0.241738721797266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064760621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99839157,0.00011098205,0.0002673488,0.00005673936,0.0000033998224,0.000003815086,0.000099658486,0.000024766134,0.0010416537],"genre_scores_gemma":[0.99907255,0.000045838246,0.0002887407,0.00004219057,0.000024570332,0.0000041420626,0.00021270027,0.0000037845562,0.00030549668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999521,0.000002032319,0.0000037677623,0.000014528408,0.000010625897,0.000016981705],"domain_scores_gemma":[0.99961036,0.000046128393,0.00013440107,0.00005252296,0.00006517938,0.000091454414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013399616,0.00013706849,0.00011273405,0.000797822,0.0002550852,0.00041015312,0.0003367184,0.000396599,0.0012609451],"category_scores_gemma":[0.00034112425,0.00011746816,0.00015399407,0.00030147252,0.00040342694,0.00037726728,0.0003928714,0.00023518963,0.00019710552],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031021755,0.00010885289,0.7976193,0.000055816075,0.00006459328,0.0024685077,0.0007995876,0.0002211313,0.18625729,0.00032942212,0.00066827406,0.011097119],"study_design_scores_gemma":[0.0000057301677,0.00004867225,0.9944853,0.0000031974987,0.000011492332,0.00083353743,0.000063231644,0.00014454557,0.0035922877,0.00004962333,0.00075844163,0.0000038614835],"about_ca_topic_score_codex":0.0025873515,"about_ca_topic_score_gemma":0.005348862,"teacher_disagreement_score":0.0025873515,"about_ca_system_score_codex":0.00026298646,"about_ca_system_score_gemma":0.000061385384,"threshold_uncertainty_score":0.0051446557},"labels":[],"label_agreement":null},{"id":"W2064846308","doi":"10.1086/592764","title":"Lithium Depletion of Nearby Young Stellar Associations","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":161,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"myr; Astrophysics; Physics; Stars; Surface gravity; Cluster (spacecraft); Open cluster; Lithium (medication); Spectral line; Abundance (ecology); Effective temperature; Star cluster; Astronomy; Chemistry; Biology; Ecology","score_opus":0.014454936282707798,"score_gpt":0.22365172641471445,"score_spread":0.20919679013200665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064846308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995005,0.000032127737,0.00012112122,0.0000028164723,4.3376184e-7,9.2245887e-7,0.00006429836,0.000013253641,0.00026457148],"genre_scores_gemma":[0.9992716,0.000019900297,0.0002365238,0.0000024540552,0.0000011239428,0.0000013989081,0.00031460728,0.000004596231,0.00014781447],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999428,0.0000042664396,0.000002912996,0.000025605621,0.000011822976,0.000012644817],"domain_scores_gemma":[0.9996792,0.00003836569,0.00010796868,0.000037272148,0.000053854732,0.000083339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001297576,0.00019472974,0.00019371843,0.0006004179,0.0004404045,0.0003911844,0.00031711522,0.00020406592,0.0006626627],"category_scores_gemma":[0.00046614572,0.00012826857,0.0001457893,0.00045592265,0.00019316068,0.0002272073,0.00032210408,0.00014052325,0.00022688581],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021205998,0.000016000115,0.9791077,0.0000140852035,0.000041546675,0.000074718504,0.0002029704,0.0019613716,0.0141626615,0.0001240615,0.00009753917,0.0039851773],"study_design_scores_gemma":[0.000005340537,0.000039870833,0.99193805,0.0000017759271,0.000016524038,0.000080493606,0.000077848665,0.004155583,0.003106521,0.00009960101,0.00047330608,0.0000050946396],"about_ca_topic_score_codex":0.007270937,"about_ca_topic_score_gemma":0.012824745,"teacher_disagreement_score":0.007270937,"about_ca_system_score_codex":0.00052006426,"about_ca_system_score_gemma":0.000114306546,"threshold_uncertainty_score":0.014457226},"labels":[],"label_agreement":null},{"id":"W2064909637","doi":"10.1086/587830","title":"The Color Bimodality in Galaxy Clusters since<i>z</i>∼ 0.9","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Bimodality; Galaxy cluster; Redshift; Galaxy; Cluster (spacecraft); Population; Astronomy; Brightest cluster galaxy; Demography","score_opus":0.009514708020669534,"score_gpt":0.21406071337972205,"score_spread":0.2045460053590525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064909637","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926166,0.00058573054,0.0001308901,0.00038118905,0.000015797512,0.0000035592514,0.0009114704,0.00004512992,0.005309565],"genre_scores_gemma":[0.9988003,0.000080690676,0.00003601147,0.00003963937,0.00001139732,0.000001840113,0.0003459931,0.000008729981,0.00067548786],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984527,0.000011973126,0.0000055290852,0.000052690946,0.000021188724,0.00006338762],"domain_scores_gemma":[0.9977731,0.00021151679,0.00060755166,0.00015034458,0.0005168912,0.00074046745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027147902,0.000085973676,0.00013271793,0.0024332786,0.0006243245,0.0011294979,0.00029533842,0.0003206435,0.005566701],"category_scores_gemma":[0.0019950685,0.0001304098,0.00012727645,0.0014303119,0.000595922,0.00052673084,0.000733301,0.0003553456,0.00081847154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020309711,0.000019606,0.9779714,0.00002041392,0.000018252767,0.000051399988,0.001012614,0.00010092521,0.0029010726,0.0009271213,0.0022170518,0.014557034],"study_design_scores_gemma":[0.0000011215398,0.0000057663437,0.99876153,0.0000032631806,0.0000024242822,0.000025177662,0.0002594469,0.000041903364,0.00007195675,0.00011028859,0.00071531854,0.0000018133968],"about_ca_topic_score_codex":0.04503106,"about_ca_topic_score_gemma":0.068717085,"teacher_disagreement_score":0.04503106,"about_ca_system_score_codex":0.0007949663,"about_ca_system_score_gemma":0.00046560724,"threshold_uncertainty_score":0.08953792},"labels":[],"label_agreement":null},{"id":"W2064915906","doi":"10.1088/0004-637x/734/1/68","title":"GALAXY CLUSTERS AT HIGH REDSHIFT AND EVOLUTION OF BRIGHTEST CLUSTER GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Redshift; Galaxy; Galaxy cluster; Cluster (spacecraft); Galaxy formation and evolution; Galaxy groups and clusters; Cosmology; Redshift survey","score_opus":0.008047730535915745,"score_gpt":0.1911787521149601,"score_spread":0.18313102157904437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064915906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992803,0.00009947095,0.00008943575,0.000012242144,9.25265e-7,0.0000022540953,0.00022131867,0.0000068912914,0.00028708583],"genre_scores_gemma":[0.99889874,0.00006247049,0.00023698366,0.000006815948,0.0000039609513,0.0000024590142,0.0005319024,0.0000046767786,0.00025200835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999777,0.000025004027,0.000007950777,0.00007690304,0.000040344123,0.000072708885],"domain_scores_gemma":[0.9988877,0.00012457655,0.0004933486,0.00010927904,0.000105368206,0.0002797778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029957865,0.00013070248,0.00020129434,0.00180597,0.00057947775,0.00065237866,0.00019482058,0.00029715846,0.0014166961],"category_scores_gemma":[0.0009487767,0.00016799616,0.00022582593,0.0013918006,0.00036945613,0.00035105553,0.00053299865,0.00026686155,0.00030515276],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056437617,0.000025915133,0.9939547,0.0000057942,0.00002434917,0.000053140582,0.00020985643,0.0003724075,0.002228581,0.00028566612,0.00017382999,0.0026093978],"study_design_scores_gemma":[0.0000011276065,0.000008268378,0.9995227,8.347787e-7,0.0000040636305,0.0000304961,0.000050059003,0.00015397804,0.00008374564,0.00004374101,0.000099280966,0.0000018063026],"about_ca_topic_score_codex":0.019326463,"about_ca_topic_score_gemma":0.023936069,"teacher_disagreement_score":0.019326463,"about_ca_system_score_codex":0.00053625467,"about_ca_system_score_gemma":0.00022395766,"threshold_uncertainty_score":0.03842789},"labels":[],"label_agreement":null},{"id":"W2064948947","doi":"10.1086/323943","title":"The Spectra of Young Protostars of Cepheus A","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Protostar; Astrophysics; Spectral line; Outflow; Flux (metallurgy); Ionization; Jet (fluid); Astronomy; Stars; Star formation; Ion","score_opus":0.008594534561719927,"score_gpt":0.236183047104071,"score_spread":0.22758851254235107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2064948947","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991762,0.00012124253,0.00013840932,0.0000057314546,0.0000030874473,0.000004388725,0.0002427897,0.000008416259,0.00029963718],"genre_scores_gemma":[0.99866426,0.000056086687,0.0002980337,0.000011621836,0.0000093756635,0.0000051348684,0.00073924265,0.0000037696987,0.00021243661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987054,0.000008873913,0.000011593782,0.000040017036,0.000039068054,0.000029878083],"domain_scores_gemma":[0.998928,0.000120076365,0.0003284874,0.00007443165,0.00020756242,0.00034141148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021527657,0.0002378538,0.0002330854,0.001230172,0.00038537086,0.00024876365,0.00017409257,0.00021581993,0.0005452886],"category_scores_gemma":[0.00053946755,0.000117589414,0.00015058134,0.00072836445,0.00017149157,0.00019397662,0.00029050215,0.00016766712,0.00020704043],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031968512,0.000076961944,0.89221597,0.000044879816,0.00007838294,0.0010367271,0.00053933467,0.00027151438,0.08598,0.00007177672,0.0003189754,0.019045759],"study_design_scores_gemma":[0.0000015530094,0.000047542188,0.99846363,0.0000010996125,0.0000048388074,0.00021762364,0.000020826888,0.00009015222,0.0009262788,0.000011491831,0.00021304129,0.0000018859583],"about_ca_topic_score_codex":0.0020645515,"about_ca_topic_score_gemma":0.003162613,"teacher_disagreement_score":0.0020645515,"about_ca_system_score_codex":0.00024926342,"about_ca_system_score_gemma":0.00009242501,"threshold_uncertainty_score":0.0041050315},"labels":[],"label_agreement":null},{"id":"W2065104492","doi":"10.1088/0004-637x/692/1/l14","title":"USING MILLIMETER VLBI TO CONSTRAIN RIAF MODELS OF SAGITTARIUS A*","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Very-long-baseline interferometry; Physics; Millimeter; Astrophysics; Accretion (finance); Supermassive black hole; Astronomy; Context (archaeology); Amplitude; Geology; Galaxy","score_opus":0.0384062206187731,"score_gpt":0.2691471271223557,"score_spread":0.23074090650358262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065104492","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98979,0.0001409067,0.0067614517,0.000088001325,0.0000052898827,0.000012405732,0.0003477726,0.00015716879,0.0026969758],"genre_scores_gemma":[0.996058,0.00004492154,0.0030670092,0.000014670347,0.0000041659714,0.0000068923973,0.00067414413,0.000014643802,0.00011570936],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999851,0.00003761166,0.000007749016,0.00004380059,0.000027337006,0.00003257378],"domain_scores_gemma":[0.9993967,0.0001173241,0.00019668936,0.00014047694,0.000060002312,0.00008874264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068121887,0.0002785834,0.00021199246,0.0005641368,0.00043890596,0.0009547012,0.00034808155,0.0003335108,0.0006185946],"category_scores_gemma":[0.0019797687,0.0002725675,0.00034436793,0.0003887105,0.00023772728,0.0006591427,0.00053716707,0.00041204915,0.00024651192],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024079485,0.00009579097,0.90853673,0.00003571894,0.00017272757,0.00014239924,0.0003379844,0.02629902,0.032099556,0.0038340352,0.00092728715,0.027277894],"study_design_scores_gemma":[0.000052961794,0.00018347557,0.83944,0.000020889172,0.0000630497,0.00017958158,0.0003465805,0.14731172,0.0037691237,0.0047808113,0.0038087661,0.000043018397],"about_ca_topic_score_codex":0.010813633,"about_ca_topic_score_gemma":0.011643228,"teacher_disagreement_score":0.010813633,"about_ca_system_score_codex":0.0009705071,"about_ca_system_score_gemma":0.00036001968,"threshold_uncertainty_score":0.021501362},"labels":[],"label_agreement":null},{"id":"W2065132163","doi":"10.1086/512767","title":"X‐Ray Supercavities in the Hydra A Cluster and the Outburst History of the Central Galaxy’s Active Nucleus","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":201,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Supermassive black hole; Astronomy; Galaxy; Solar mass; Outflow; Cooling flow; Brightest cluster galaxy; Black hole (networking); Active galactic nucleus; RADIUS; Surface brightness; Galaxy cluster","score_opus":0.00965013071590936,"score_gpt":0.20550800794866209,"score_spread":0.19585787723275272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065132163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994444,0.000027920785,0.000008134724,0.000016124595,0.0000010031731,8.2782896e-7,0.00009883167,0.000003264378,0.00039949204],"genre_scores_gemma":[0.9995708,0.000028375125,0.00002238445,0.000006541295,0.0000039794627,0.0000012639358,0.00018081373,0.0000029189412,0.0001830095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999304,0.0000064538335,0.0000034707746,0.00002466504,0.0000101215655,0.000024955641],"domain_scores_gemma":[0.9993925,0.000070714406,0.00019523162,0.000055404635,0.00005924321,0.00022692946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013204337,0.00012010097,0.00014344003,0.00078201975,0.00059244025,0.0007505696,0.00021055818,0.00017291878,0.0011652813],"category_scores_gemma":[0.00048498408,0.000146525,0.00014892862,0.0005448119,0.00046105045,0.0002648106,0.00070608925,0.00019393725,0.00021820045],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016905463,0.000025749387,0.9906483,0.000008452926,0.000029027311,0.0004083017,0.0007800281,0.00022118085,0.004969413,0.00019670208,0.00028788418,0.0022559115],"study_design_scores_gemma":[0.0000010244605,0.000007179226,0.99941313,0.0000011396544,0.0000032727917,0.000058808626,0.00018745124,0.00008974397,0.00007272708,0.000026452477,0.00013697181,0.000002101379],"about_ca_topic_score_codex":0.019462038,"about_ca_topic_score_gemma":0.021915272,"teacher_disagreement_score":0.019462038,"about_ca_system_score_codex":0.00057241286,"about_ca_system_score_gemma":0.00018949053,"threshold_uncertainty_score":0.03869754},"labels":[],"label_agreement":null},{"id":"W2065221900","doi":"10.1086/308984","title":"The Primordial Helium Abundance: Toward Understanding and Removing the Cosmic Scatter in the<i>dY/dZ</i>Relation","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Metallicity; Physics; Astrophysics; Photoionization; Helium; Stars; Ionization; Abundance (ecology); Doubly ionized oxygen; Effective temperature; Line (geometry); Atomic physics; Ion; Biology","score_opus":0.018709295203485084,"score_gpt":0.22980351804858332,"score_spread":0.21109422284509824,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065221900","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90431076,0.0015656879,0.08938167,0.00045309693,0.00002674667,0.0000063986395,0.0003273845,0.00046555398,0.0034627274],"genre_scores_gemma":[0.98961943,0.00034231995,0.009409496,0.000047623307,0.000018707178,0.0000031741556,0.00022066961,0.00008118755,0.00025736177],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997458,0.00007901981,0.000009288978,0.000072431314,0.00006778346,0.000025665919],"domain_scores_gemma":[0.9979925,0.0008021633,0.00045095186,0.00052990264,0.00012498924,0.00009950291],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010900431,0.00033141763,0.000336694,0.0006667913,0.00021861796,0.0008982333,0.00062468904,0.00030032042,0.0005358671],"category_scores_gemma":[0.005340722,0.00018165975,0.00029839028,0.00063790794,0.00052849454,0.000992442,0.0006406252,0.0004808781,0.00018775267],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031046112,0.0000754947,0.73900914,0.00017416147,0.00031204236,0.00042736638,0.0005393673,0.104171135,0.033670973,0.028563255,0.0017672849,0.09097932],"study_design_scores_gemma":[0.000047253376,0.000093383394,0.33393633,0.0000377343,0.000102588696,0.00045257996,0.00015859016,0.5903328,0.028941393,0.038652156,0.0071642464,0.0000808216],"about_ca_topic_score_codex":0.0042124945,"about_ca_topic_score_gemma":0.0037692077,"teacher_disagreement_score":0.0042124945,"about_ca_system_score_codex":0.0004717496,"about_ca_system_score_gemma":0.00028123418,"threshold_uncertainty_score":0.008375943},"labels":[],"label_agreement":null},{"id":"W2065263003","doi":"10.1088/0004-637x/743/1/68","title":"STRONG GRAVITATIONAL LENS MODELING WITH SPATIALLY VARIANT POINT-SPREAD FUNCTIONS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Point spread function; Deconvolution; Gravitational lens; Lens (geology); Context (archaeology); Optical transfer function; Pixel; Point (geometry); Strong gravitational lensing; Computer science; Optics; Point source; Code (set theory); Algorithm; Position (finance); Source code; Physics; Mathematics; Astrophysics; Geometry; Geology","score_opus":0.029358620219415637,"score_gpt":0.22273738691831826,"score_spread":0.19337876669890264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065263003","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.044945918,0.000071457536,0.9533668,0.00009016778,0.0000083255245,0.00001613605,0.00003854257,0.00016941887,0.0012931523],"genre_scores_gemma":[0.75531155,0.00024135942,0.2396323,0.000052876672,0.0000272393,0.00005974207,0.00012197578,0.0000897675,0.0044631003],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997844,0.000060299848,0.000011541203,0.000041602947,0.00008110479,0.00002093029],"domain_scores_gemma":[0.9992778,0.00035840066,0.00014345285,0.00008352526,0.00010752281,0.000029362654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007794942,0.00065145415,0.0003436902,0.00040854543,0.00029097975,0.00072418194,0.0012887991,0.0009157538,0.0006437712],"category_scores_gemma":[0.0024773038,0.00032676145,0.0006683726,0.00044833185,0.00064848113,0.0011862698,0.00081901415,0.0007573766,0.00017442704],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002882079,0.000012324717,0.00070369546,0.000016928236,0.000019471687,0.0000392635,0.000052316274,0.96446157,0.0036532995,0.022506697,0.00017216124,0.008333551],"study_design_scores_gemma":[0.000002571412,0.000005310026,0.000108142194,9.0466193e-7,0.0000023230264,0.000008548785,0.0000033995184,0.9965958,0.0006905501,0.002444616,0.0001334568,0.0000043610903],"about_ca_topic_score_codex":0.009284219,"about_ca_topic_score_gemma":0.0067174355,"teacher_disagreement_score":0.009284219,"about_ca_system_score_codex":0.0007332825,"about_ca_system_score_gemma":0.00082927034,"threshold_uncertainty_score":0.018460393},"labels":[],"label_agreement":null},{"id":"W2065263870","doi":"10.1086/378846","title":"The Origin of Jovian Planets in Protostellar Disks: The Role of Dead Zones","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Planet; Astrophysics; Cosmic ray; Accretion (finance); Planetesimal; Jovian; Planetary migration; Protoplanetary disk; Formation and evolution of the Solar System; Astronomy; Magnetorotational instability; Planetary system; Gas giant; Exoplanet; Ionization; Plasma; Magnetohydrodynamics","score_opus":0.008005333597568245,"score_gpt":0.23305909159521992,"score_spread":0.22505375799765168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065263870","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99532473,0.001125609,0.0023707703,0.000050750514,0.0000032528171,0.0000043746527,0.00006971457,0.00002570736,0.001025184],"genre_scores_gemma":[0.9992465,0.00014203832,0.0004345705,0.0000045596444,0.0000025493441,0.0000016401685,0.00003114757,0.000007081606,0.00012998741],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992335,0.000012777599,0.000006073554,0.000023090468,0.000012701168,0.000021949105],"domain_scores_gemma":[0.99937207,0.00016788699,0.0001924375,0.00006831353,0.00004821101,0.0001511648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021516945,0.00031213573,0.00027064892,0.00063409976,0.0006194341,0.0014546611,0.00087620213,0.0006784768,0.0005270841],"category_scores_gemma":[0.0010384123,0.00023666932,0.00026028865,0.00030811885,0.0008783102,0.0011611577,0.0009744425,0.00030605073,0.0001934421],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015330812,0.00014841522,0.60329074,0.0006344372,0.00015354346,0.0023157292,0.0029188148,0.046354886,0.26047692,0.04885396,0.0005974577,0.032722034],"study_design_scores_gemma":[0.00011106272,0.0004076337,0.77033764,0.000103027705,0.0001743598,0.0036042621,0.0027149506,0.105956405,0.0652971,0.042982627,0.008176187,0.00013466699],"about_ca_topic_score_codex":0.001079523,"about_ca_topic_score_gemma":0.00072673993,"teacher_disagreement_score":0.0014546611,"about_ca_system_score_codex":0.00048940955,"about_ca_system_score_gemma":0.000105754,"threshold_uncertainty_score":0.0035509467},"labels":[],"label_agreement":null},{"id":"W2065392390","doi":"10.1086/308225","title":"The Core Density of Dark Matter Halos: A Critical Challenge to the ΛCDM Paradigm?","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Dark matter; Dark matter halo; Galaxy rotation curve; Cold dark matter; Galaxy; Halo; Galaxy formation and evolution; Milky Way; Astronomy; Baryonic dark matter","score_opus":0.01101468776847218,"score_gpt":0.2333710258484933,"score_spread":0.22235633808002114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065392390","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.940146,0.0032949578,0.022128856,0.015432655,0.00011473037,0.000021869022,0.00038837406,0.00015844965,0.018314045],"genre_scores_gemma":[0.9954673,0.00058710837,0.0028845177,0.0003780207,0.00009814031,0.0000105716435,0.00003957101,0.000024442268,0.0005102445],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998604,0.00005446732,0.00000460144,0.000040479223,0.000022486376,0.00001748002],"domain_scores_gemma":[0.9982528,0.00089830486,0.0002666423,0.00020441714,0.00017819213,0.00019965785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012029444,0.0002454268,0.0004227627,0.0005597448,0.0005655128,0.0018806672,0.0012359292,0.0007968738,0.0015491763],"category_scores_gemma":[0.0079296995,0.00023019507,0.00018341205,0.0005404964,0.0014492212,0.0029598696,0.0009490539,0.0005297392,0.0002680562],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047770332,0.0001169759,0.16304201,0.00024983872,0.00018332055,0.0005138548,0.001561157,0.08237607,0.006004315,0.66601056,0.0077467724,0.07171741],"study_design_scores_gemma":[0.00013279656,0.00007906575,0.05194682,0.00014697066,0.000051807212,0.00021427586,0.0011787344,0.31307364,0.0015343692,0.622791,0.008767695,0.00008282211],"about_ca_topic_score_codex":0.0069961688,"about_ca_topic_score_gemma":0.0065248357,"teacher_disagreement_score":0.0069961688,"about_ca_system_score_codex":0.00097166735,"about_ca_system_score_gemma":0.00047632676,"threshold_uncertainty_score":0.01391089},"labels":[],"label_agreement":null},{"id":"W2065424285","doi":"10.1086/518433","title":"Fragmentation of Gravitationally Unstable Gaseous Protoplanetary Disks with Radiative Transfer","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":175,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Opacity; Radiative transfer; Fragmentation (computing); Convection; Protoplanetary disk; Metallicity; Thin disk; Planet; Astronomy; Stars; Mechanics; Optics","score_opus":0.006874971143914495,"score_gpt":0.230719980570247,"score_spread":0.2238450094263325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065424285","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952187,0.00006386599,0.0014994612,0.000089131725,0.000014144616,0.00003168363,0.00029939515,0.00013416493,0.0026493983],"genre_scores_gemma":[0.9971716,0.000038232392,0.001885184,0.000047933954,0.000009891957,0.00002512622,0.0003198715,0.000041202264,0.00046103197],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998416,0.000030663858,0.0000067069445,0.000019432411,0.000037410293,0.00006421347],"domain_scores_gemma":[0.9993044,0.0003132599,0.000096134965,0.00004921077,0.000067076675,0.0001699538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000305841,0.0007172682,0.0007780871,0.00040975472,0.00064183376,0.00088264246,0.0013686892,0.0011159765,0.0013648908],"category_scores_gemma":[0.0015954906,0.00039096037,0.0008656692,0.00048573676,0.0010310502,0.00049184,0.0008250629,0.000776821,0.0001501754],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005055336,0.0002533889,0.018337527,0.00007640208,0.00015546002,0.0010683959,0.00032958316,0.9664193,0.0070305234,0.0019655298,0.0005532089,0.0033052224],"study_design_scores_gemma":[0.00015646892,0.00012466242,0.004782094,0.0000064463743,0.000016714372,0.00009325329,0.000082460494,0.9922552,0.0015234147,0.0006361831,0.00030943466,0.000013555205],"about_ca_topic_score_codex":0.015791511,"about_ca_topic_score_gemma":0.005269731,"teacher_disagreement_score":0.015791511,"about_ca_system_score_codex":0.0010718972,"about_ca_system_score_gemma":0.0008061693,"threshold_uncertainty_score":0.03139919},"labels":[],"label_agreement":null},{"id":"W2065652673","doi":"10.1088/0004-637x/756/1/24","title":"SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC). VI. THE PLANETARY-MASS DOMAIN OF NGC 1333","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Gravitational microlensing; Brown dwarf; Stars; Cluster (spacecraft); Population; Stellar classification; Low Mass; Star cluster","score_opus":0.007920163067024602,"score_gpt":0.21656186008221667,"score_spread":0.20864169701519208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065652673","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990513,0.00007849229,0.00011058445,0.00000840277,0.0000012055764,0.0000034875393,0.0002808907,0.000013742725,0.00045194075],"genre_scores_gemma":[0.99850637,0.000058837133,0.00028924024,0.00000767398,0.0000034869706,0.000006025709,0.00087213225,0.000004166927,0.0002521641],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991274,0.000008766819,0.000007679982,0.000021471857,0.00002274636,0.00002662133],"domain_scores_gemma":[0.9996111,0.000041281677,0.00016354569,0.0000342662,0.00004471099,0.00010522722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013097946,0.00014066053,0.00016383671,0.00097645586,0.00044129434,0.000336526,0.00016462407,0.00013624209,0.0014954204],"category_scores_gemma":[0.000331791,0.000063123945,0.00016891428,0.0011830098,0.00025570713,0.00016222066,0.0005727649,0.00013999724,0.0002696714],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013855674,0.000015282498,0.9836669,0.000019591438,0.000015257771,0.00022102782,0.0003263587,0.00017389338,0.006960536,0.00018956568,0.0003820843,0.007891075],"study_design_scores_gemma":[0.0000017677955,0.000016064056,0.9985543,0.0000019268055,0.0000047510357,0.00026831988,0.00015250458,0.00017470102,0.00028744608,0.000031299624,0.00050531875,0.0000016218461],"about_ca_topic_score_codex":0.017006652,"about_ca_topic_score_gemma":0.03593327,"teacher_disagreement_score":0.017006652,"about_ca_system_score_codex":0.00032100966,"about_ca_system_score_gemma":0.00023568304,"threshold_uncertainty_score":0.033815324},"labels":[],"label_agreement":null},{"id":"W2065656945","doi":"10.1086/432882","title":"Possible Optical Detection of the Anomalous X-Ray Pulsar CXOU J010043.1-721134","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Pulsar; Hubble space telescope; Large Magellanic Cloud; Hubble Deep Field South; Ultraviolet; Spitzer Space Telescope; Neutron star; Space (punctuation); Identification (biology)","score_opus":0.008295303846678946,"score_gpt":0.21843034432008904,"score_spread":0.21013504047341008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065656945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978522,0.00013810865,0.00024979643,0.000113482056,0.000021543625,0.0000032596934,0.00010064593,0.000020982403,0.0014999796],"genre_scores_gemma":[0.99896395,0.000045388755,0.00037860652,0.00004217601,0.000022287366,0.000003412696,0.00020490076,0.0000026127598,0.00033662273],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990416,0.000013373783,0.000006249984,0.000022558845,0.000018925513,0.000034757533],"domain_scores_gemma":[0.9994698,0.00009817275,0.00021721065,0.000044369215,0.00006327281,0.000107131345],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022499291,0.00017919345,0.0001936911,0.00063774746,0.00063973083,0.00052138325,0.00027721387,0.0007340708,0.0020757003],"category_scores_gemma":[0.00074669684,0.0001473001,0.000108339475,0.0005614461,0.00032386847,0.00026323932,0.00041367716,0.00032156927,0.0002729305],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062328164,0.0001716601,0.848898,0.000098139644,0.00007386178,0.0035958723,0.00042243162,0.00019355486,0.119187005,0.0017689579,0.0014498747,0.02351736],"study_design_scores_gemma":[0.00003811928,0.0001790223,0.98270124,0.000015260928,0.000054686472,0.0033464693,0.00026264507,0.0006867661,0.007492155,0.0006527072,0.004555507,0.000015470903],"about_ca_topic_score_codex":0.0016987885,"about_ca_topic_score_gemma":0.00354648,"teacher_disagreement_score":0.0020757003,"about_ca_system_score_codex":0.000261509,"about_ca_system_score_gemma":0.00017115341,"threshold_uncertainty_score":0.006943941},"labels":[],"label_agreement":null},{"id":"W2065691631","doi":"10.1088/0004-637x/734/2/99","title":"MORPHOLOGICALLY IDENTIFIED MERGING GALAXIES IN THE SWIRE FIELDS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Astrophysics; Galaxy; Redshift; Physics; Luminosity; Star formation; Galaxy merger; Astronomy; Luminous infrared galaxy; Galaxy formation and evolution","score_opus":0.01769519375891486,"score_gpt":0.21928167687338274,"score_spread":0.20158648311446786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065691631","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995813,0.000045173052,0.00003926361,0.0000036826173,2.900564e-7,0.0000019169026,0.00011685106,0.000004553319,0.00020707969],"genre_scores_gemma":[0.99762505,0.000053874825,0.00036308798,0.000008408068,0.0000037954378,0.0000038063702,0.0017185452,0.0000043599525,0.00021908527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975675,0.00003463175,0.00001781862,0.00006749071,0.00005616154,0.000067145775],"domain_scores_gemma":[0.99863845,0.00019414925,0.00072075997,0.00013907028,0.0001294058,0.00017824193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005977819,0.00025800592,0.00027986174,0.0025024917,0.00043054108,0.00043385703,0.000298604,0.00020124369,0.0007596619],"category_scores_gemma":[0.0012263872,0.00019740005,0.00024961776,0.0010418901,0.0002342421,0.00037291684,0.00050597114,0.00013351598,0.000184141],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014769936,0.000060227485,0.98571485,0.000013757164,0.00006968644,0.00017487239,0.00049325393,0.00042276882,0.0064025745,0.0002116194,0.00015704577,0.0061316444],"study_design_scores_gemma":[0.0000036492988,0.000016519287,0.99875116,0.0000023487028,0.000011224029,0.000093646166,0.00008006063,0.00044841983,0.00033879993,0.000019796165,0.000231991,0.0000022993372],"about_ca_topic_score_codex":0.009072095,"about_ca_topic_score_gemma":0.017412102,"teacher_disagreement_score":0.009072095,"about_ca_system_score_codex":0.0004614213,"about_ca_system_score_gemma":0.00015658351,"threshold_uncertainty_score":0.01803857},"labels":[],"label_agreement":null},{"id":"W2065726607","doi":"10.1086/498208","title":"Galaxy Rotation Curves without Nonbaryonic Dark Matter","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":325,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Perimeter Institute","funders":"","keywords":"Physics; Galaxy rotation curve; Astrophysics; Modified Newtonian dynamics; Dark matter; Galaxy; Surface brightness fluctuation; Elliptical galaxy; Fundamental plane (elliptical galaxies); Surface brightness; Satellite galaxy; Luminosity; Astronomy; Dark matter halo; Brightest cluster galaxy; Lenticular galaxy; Galaxy formation and evolution","score_opus":0.004473508686395247,"score_gpt":0.2310393521410076,"score_spread":0.22656584345461234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065726607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94737077,0.00046769276,0.040559474,0.00011423918,0.000020189542,0.00002826588,0.0013162462,0.0004962484,0.009626878],"genre_scores_gemma":[0.99463034,0.00013259958,0.003897627,0.0000064911433,0.00000956639,0.0000070800243,0.0008095611,0.000035724515,0.00047101217],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999064,0.00002675195,0.0000058993764,0.000024190209,0.00001678265,0.000019932872],"domain_scores_gemma":[0.9993304,0.00016982715,0.00015585494,0.0002005403,0.000081457314,0.00006197932],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027387202,0.00037031528,0.00024250991,0.00084331224,0.00012430806,0.00031871677,0.00018630321,0.00016563224,0.002008377],"category_scores_gemma":[0.0027303773,0.000069829075,0.00028188998,0.0007513275,0.0002120058,0.00030448264,0.00025732518,0.00017617778,0.00077544304],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007479979,0.000066751636,0.358827,0.00020914714,0.0002086274,0.00057729764,0.0005375999,0.35223606,0.017021561,0.074649915,0.0030176044,0.19190048],"study_design_scores_gemma":[0.000080855854,0.00027531985,0.3931846,0.00005090191,0.000058473248,0.0011101973,0.00015087391,0.5358506,0.005730475,0.04371386,0.019739166,0.000054705113],"about_ca_topic_score_codex":0.0018695688,"about_ca_topic_score_gemma":0.0018762178,"teacher_disagreement_score":0.002008377,"about_ca_system_score_codex":0.00022786441,"about_ca_system_score_gemma":0.00009290757,"threshold_uncertainty_score":0.006718695},"labels":[],"label_agreement":null},{"id":"W2065759510","doi":"10.1088/0004-637x/782/1/50","title":"ON THE KINEMATIC SEPARATION OF FIELD AND CLUSTER STARS ACROSS THE BULGE GLOBULAR NGC 6528","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Open cluster; Bulge; Astronomy; Red-giant branch; Photometry (optics); Horizontal branch; Stars; Star cluster; Advanced Camera for Surveys; Proper motion; Hubble space telescope","score_opus":0.008171643214031936,"score_gpt":0.24879793099627834,"score_spread":0.2406262877822464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065759510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991571,0.00009846509,0.00009918116,0.000009716543,0.0000018414903,8.451307e-7,0.00010436072,0.000005168726,0.0005234047],"genre_scores_gemma":[0.9994313,0.000032719225,0.0001356415,0.0000035823407,0.000002099801,0.0000012637812,0.0002756882,0.0000022922957,0.00011527916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999043,0.000009129213,0.000004911389,0.000046658577,0.000017249487,0.000017753513],"domain_scores_gemma":[0.9996055,0.000063945205,0.00012311383,0.000046657668,0.00007100657,0.0000898109],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001809025,0.00018000139,0.00011629522,0.0008983792,0.00023696781,0.0003999639,0.00024393236,0.000118782766,0.0006775038],"category_scores_gemma":[0.0007452005,0.00008542247,0.00009001665,0.00052060484,0.00025625527,0.00021644992,0.0005612396,0.000114118244,0.00017955227],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012397533,0.000016441449,0.97921926,0.000015160937,0.000026197351,0.00012205303,0.00034862958,0.00069416245,0.007840094,0.00029425343,0.00019103772,0.011108559],"study_design_scores_gemma":[0.0000028988009,0.00001892689,0.9986008,0.0000044177627,0.000007259007,0.00005783316,0.00009920245,0.00049089553,0.00021683269,0.00008123646,0.0004175492,0.0000021291087],"about_ca_topic_score_codex":0.013440845,"about_ca_topic_score_gemma":0.027899591,"teacher_disagreement_score":0.013440845,"about_ca_system_score_codex":0.00040102375,"about_ca_system_score_gemma":0.00018697498,"threshold_uncertainty_score":0.026725233},"labels":[],"label_agreement":null},{"id":"W2065914873","doi":"10.1086/308659","title":"The Globular Cluster Systems in the Coma Ellipticals. II. Metallicity Distribution and Radial Structure in NGC 4874 and Implications for Galaxy Formation","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Queen's University; Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Astronomy; Brightest cluster galaxy; Elliptical galaxy; Interacting galaxy; Lenticular galaxy; Dwarf galaxy; Galaxy; Galaxy cluster; Galaxy merger","score_opus":0.0060249889289012044,"score_gpt":0.21482702048822985,"score_spread":0.20880203155932864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065914873","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968412,0.00027921417,0.000054566357,0.00008788672,0.0000018290718,0.0000026236949,0.000078870675,0.000007454557,0.0026463745],"genre_scores_gemma":[0.9994092,0.000085986656,0.00005694037,0.000008880195,0.0000033655956,0.0000013964109,0.00006247357,6.535696e-7,0.00037127893],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999471,0.000007870526,0.0000018338854,0.0000059885165,0.000008892205,0.000028290193],"domain_scores_gemma":[0.9998734,0.000012128034,0.000041254447,0.000006823704,0.000017864819,0.000048562637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000066452,0.00011288379,0.00007420053,0.0008475383,0.0005856756,0.00048754492,0.00016297805,0.00017410419,0.0019833767],"category_scores_gemma":[0.00025354626,0.000087823915,0.000061900086,0.0005543647,0.0007050443,0.00032464686,0.00035609287,0.00012487012,0.0002542199],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017307943,0.00003651567,0.96062785,0.000029055247,0.00002112474,0.0007709638,0.0012204674,0.00079261156,0.01172794,0.005820043,0.0013982303,0.017382026],"study_design_scores_gemma":[0.0000024379701,0.000017006027,0.99710256,0.000003388759,0.0000039975257,0.00018217532,0.00053080416,0.00022979887,0.00016328268,0.00047355087,0.0012888134,0.0000021170486],"about_ca_topic_score_codex":0.034232922,"about_ca_topic_score_gemma":0.06458672,"teacher_disagreement_score":0.034232922,"about_ca_system_score_codex":0.0010768109,"about_ca_system_score_gemma":0.00026813368,"threshold_uncertainty_score":0.06806731},"labels":[],"label_agreement":null},{"id":"W2065920880","doi":"10.1086/423922","title":"The Effect of Neutron Star Gravitational Binding Energy on Gravitational Radiation–driven Mass‐Transfer Binaries","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Neutron star; Gravitational redshift; Astrophysics; Baryon; Gravitational energy; Redshift; Gravitational binding energy; Gravitational wave; Angular momentum; Astronomy; Classical mechanics; Galaxy","score_opus":0.006249771383227012,"score_gpt":0.27527049133319076,"score_spread":0.26902071994996374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065920880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971367,0.000116813666,0.0004997789,0.0001105494,0.000014692427,0.0000025847157,0.000020139705,0.00003688899,0.0020617286],"genre_scores_gemma":[0.9994981,0.00003801674,0.0000726859,0.000024734496,0.0000043059936,0.0000014171967,0.000016480151,0.000009788771,0.0003344843],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99986744,0.00003096334,0.0000068299787,0.000017797714,0.000026425963,0.000050515875],"domain_scores_gemma":[0.999019,0.00042538223,0.00021426995,0.000076927594,0.00005582252,0.00020849674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006033455,0.0002827513,0.0005119716,0.00040236823,0.0009074334,0.0009994655,0.0005361489,0.0005565295,0.0032243042],"category_scores_gemma":[0.0029739637,0.00026108426,0.00021153109,0.0002836123,0.0006639931,0.0006687288,0.001287661,0.0008891247,0.00031359072],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00844973,0.0014461613,0.14670089,0.00032775465,0.00042119622,0.0024154843,0.0011445027,0.3696851,0.31962708,0.1043437,0.0026607946,0.04277758],"study_design_scores_gemma":[0.0007207976,0.0014934227,0.25376064,0.00004686787,0.00024111998,0.00093622005,0.0005739007,0.6236628,0.06276841,0.05313379,0.0024734994,0.00018853253],"about_ca_topic_score_codex":0.0026024487,"about_ca_topic_score_gemma":0.0019358366,"teacher_disagreement_score":0.0032243042,"about_ca_system_score_codex":0.0008550554,"about_ca_system_score_gemma":0.0003730637,"threshold_uncertainty_score":0.010786414},"labels":[],"label_agreement":null},{"id":"W2065921942","doi":"10.1088/0004-637x/785/1/31","title":"DETAILED NUMERICAL INVESTIGATION OF THE BOHM LIMIT IN COSMIC RAY DIFFUSION THEORY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Mean free path; Gyroradius; Diffusion; Cosmic ray; RADIUS; Limit (mathematics); Anomalous diffusion; Field (mathematics); Turbulence; Test particle; Computational physics; Magnetic field; Mean field theory; Classical mechanics; Astrophysics; Quantum mechanics; Mechanics; Scattering; Mathematical analysis","score_opus":0.00501519568108965,"score_gpt":0.19640694259561642,"score_spread":0.19139174691452676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065921942","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8785733,0.0018075741,0.06780444,0.0013905753,0.0001305467,0.00010016736,0.0006778325,0.00050192984,0.049013652],"genre_scores_gemma":[0.97889173,0.00026281577,0.018052706,0.00010871196,0.000025178882,0.00009401454,0.00030157444,0.00009186894,0.0021712752],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99973124,0.00009555525,0.000014606823,0.000024996065,0.000077948804,0.000055608878],"domain_scores_gemma":[0.9985942,0.0009236855,0.0001215316,0.0001013691,0.00017786183,0.000081342594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009308161,0.00042605735,0.000719962,0.00083385693,0.00091563904,0.0008529343,0.00085578236,0.0009789127,0.0026482844],"category_scores_gemma":[0.0042800168,0.00022113367,0.00044844468,0.00074952753,0.0010158902,0.0010570684,0.000866248,0.00074557343,0.00014616706],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001087761,0.00009614905,0.0053503425,0.00012836052,0.000041824573,0.000294494,0.00024960915,0.8902815,0.003547551,0.094450586,0.0012055769,0.00424526],"study_design_scores_gemma":[0.000010627664,0.000011800629,0.00046318464,0.000008187975,0.0000041394405,0.000016097156,0.000021979426,0.9925351,0.0002490055,0.0063746716,0.00029843353,0.0000066936745],"about_ca_topic_score_codex":0.009014433,"about_ca_topic_score_gemma":0.004747538,"teacher_disagreement_score":0.009014433,"about_ca_system_score_codex":0.0010311897,"about_ca_system_score_gemma":0.00085769146,"threshold_uncertainty_score":0.017923892},"labels":[],"label_agreement":null},{"id":"W2065983520","doi":"10.1086/431898","title":"Constraints on Inner Disk Evolution Timescales: A Disk Census of the η Chamaeleontis Young Cluster","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Stars; Physics; Planet; Photometry (optics); Astronomy; Astrophysics; Debris disk; Sky; Infrared excess; Observatory; Accretion (finance); Star formation; Planetary system","score_opus":0.006451568999428854,"score_gpt":0.220994310938558,"score_spread":0.21454274193912914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2065983520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918,0.00004144964,0.00004080251,0.000007990164,6.172587e-7,0.0000026701646,0.0003140617,0.0000025625095,0.00040990365],"genre_scores_gemma":[0.9987087,0.000033909713,0.00015015385,0.000005510137,0.000002376734,0.000003190115,0.00083167554,0.000002066879,0.00026243372],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992394,0.0000055986934,0.0000050786953,0.000029142375,0.000014459759,0.000021759686],"domain_scores_gemma":[0.99954164,0.00004351267,0.0001469263,0.000043410044,0.000055307995,0.00016923326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023452837,0.00014167427,0.00015445171,0.0009359752,0.0005258429,0.0003842593,0.00022549674,0.00014221133,0.0012404261],"category_scores_gemma":[0.000476443,0.00009035713,0.000092708266,0.00066429947,0.00023386585,0.00023094824,0.00047507999,0.00010501598,0.00029086103],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008218492,0.000016231068,0.9840226,0.000018420382,0.00001155334,0.00012163633,0.0006833297,0.0001515077,0.010252665,0.00008671074,0.00015122925,0.0044019287],"study_design_scores_gemma":[0.0000012194607,0.000015135218,0.9988599,0.0000011418698,0.0000029367636,0.00006702465,0.00016384397,0.00009036639,0.00022577394,0.000014902544,0.00055627985,0.0000015237226],"about_ca_topic_score_codex":0.01845002,"about_ca_topic_score_gemma":0.05190849,"teacher_disagreement_score":0.01845002,"about_ca_system_score_codex":0.00050709397,"about_ca_system_score_gemma":0.0003244612,"threshold_uncertainty_score":0.036685288},"labels":[],"label_agreement":null},{"id":"W2066043890","doi":"10.1086/374660","title":"The Absorption and Emission Kinematics in the<i>z</i> = 0.7450 Mg<scp>ii</scp>Absorber toward Q1331+17","year":2003,"lang":"zh","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Galaxy rotation curve; Quasar; Astronomy; Galaxy formation and evolution","score_opus":0.010100850769635393,"score_gpt":0.21979701207280217,"score_spread":0.20969616130316676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066043890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951321,0.00008925725,0.00026192292,0.00010067335,0.0000020186455,0.0000037200027,0.00035228342,0.00005849844,0.003999512],"genre_scores_gemma":[0.99761766,0.000039299615,0.00022269676,0.00003094108,0.0000040022805,0.0000039704187,0.00046111597,0.000022169434,0.001598075],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996006,0.000002420938,8.2674484e-7,0.000013452818,0.0000070043016,0.000016220914],"domain_scores_gemma":[0.99986184,0.000017722125,0.000050991526,0.00000759115,0.000021752694,0.00004004555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000086954584,0.00013447527,0.000105887,0.000850419,0.0004059641,0.00045098382,0.00021127754,0.00023147225,0.0031082828],"category_scores_gemma":[0.0001391427,0.00018015111,0.0001373198,0.00052642287,0.00019062877,0.0002556491,0.00035995842,0.0002386684,0.0005844234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060504896,0.00013459586,0.68774694,0.000035363097,0.000047421254,0.0005863408,0.00083299313,0.0006771921,0.28667977,0.0014108587,0.001972308,0.01927121],"study_design_scores_gemma":[0.000008695602,0.000026942564,0.9937575,0.000003628311,0.000015136862,0.00010223148,0.00017187822,0.00085950666,0.0037575522,0.00013010898,0.0011630616,0.0000037324708],"about_ca_topic_score_codex":0.01382273,"about_ca_topic_score_gemma":0.017060384,"teacher_disagreement_score":0.01382273,"about_ca_system_score_codex":0.0004446145,"about_ca_system_score_gemma":0.00013899882,"threshold_uncertainty_score":0.027484536},"labels":[],"label_agreement":null},{"id":"W2066087926","doi":"10.1086/527462","title":"Quasar Broad Absorption Line Variability on Multiyear Timescales","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Quasar; QSOS; Astrophysics; Variation (astronomy); Photoionization; Physics; Absorption (acoustics); Absorption spectroscopy; Outflow; Equivalent width; Line (geometry); Emission spectrum; Spectral line; Astronomy; Optics; Geometry; Galaxy; Meteorology; Ionization","score_opus":0.011590112691338209,"score_gpt":0.22313042166253336,"score_spread":0.21154030897119513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066087926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989242,0.000051491996,0.00040561194,0.000008471805,0.0000011880958,0.000002930308,0.00035010313,0.000012117791,0.00024384724],"genre_scores_gemma":[0.99936146,0.0000134048205,0.00019790561,0.0000027560818,0.000002711025,0.0000042955658,0.00035526283,0.0000020970385,0.000060103284],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974614,0.000057474674,0.00002069702,0.000071659066,0.000059109854,0.000044829845],"domain_scores_gemma":[0.99641955,0.0006224285,0.0020785085,0.00026681338,0.00031261484,0.00030009303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009861314,0.00015384966,0.00020954378,0.0020080102,0.000198055,0.0005758571,0.00022116426,0.00018982508,0.00070338463],"category_scores_gemma":[0.0030659954,0.00009357727,0.00019906407,0.0012111069,0.00024982184,0.00061781623,0.000566762,0.00025428654,0.00012239603],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000411097,0.000022935938,0.98956877,0.000010729598,0.00007541103,0.00003685559,0.00018513564,0.00097340764,0.0035060125,0.0002551441,0.00009532148,0.0052293013],"study_design_scores_gemma":[7.8239043e-7,0.000029010105,0.99878126,9.4109794e-7,0.0000051205734,0.000045096705,0.00006074158,0.00071918615,0.00014582797,0.00008911156,0.000119388285,0.0000035069922],"about_ca_topic_score_codex":0.0017359474,"about_ca_topic_score_gemma":0.002368116,"teacher_disagreement_score":0.0020080102,"about_ca_system_score_codex":0.00022730285,"about_ca_system_score_gemma":0.000073178526,"threshold_uncertainty_score":0.0052152276},"labels":[],"label_agreement":null},{"id":"W2066153886","doi":"10.1086/321503","title":"A Submillimeter Study of the Star‐forming Region NGC 7129","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Astrophysics; Physics; Protostar; Molecular cloud; Infrared; Star formation; Spectral line; Astronomy; Stars","score_opus":0.018427777768807475,"score_gpt":0.24368811488683806,"score_spread":0.2252603371180306,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066153886","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99846303,0.000057606063,0.000086421125,0.000009916214,0.0000011857219,0.000004000339,0.00020546804,0.000008123156,0.0011642916],"genre_scores_gemma":[0.9984926,0.00005561291,0.00026766388,0.000014012793,0.0000030245515,0.000004383774,0.0006004949,0.0000034689617,0.0005586788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999943,0.000004062305,0.0000017371453,0.000016101394,0.00001548732,0.00001950323],"domain_scores_gemma":[0.99987864,0.00001296772,0.000025163888,0.000012580558,0.000019937546,0.00005071111],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006311185,0.00015231554,0.00014194836,0.00047056618,0.0004368942,0.00022194184,0.00012902386,0.00013742814,0.001176338],"category_scores_gemma":[0.00011844853,0.00010831096,0.00010939316,0.00037778463,0.000099377256,0.00013103655,0.00021008591,0.00016257913,0.0003443148],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002067901,0.00018213381,0.746287,0.00007058644,0.000060264523,0.0022834176,0.0022096275,0.0011477991,0.2226705,0.0003069615,0.0010872455,0.023487745],"study_design_scores_gemma":[0.0000017401528,0.000021638354,0.9982906,0.0000023616901,0.0000025272732,0.0002531422,0.00008945486,0.00016154817,0.0005436075,0.000013890859,0.00061731384,0.000002124444],"about_ca_topic_score_codex":0.018419145,"about_ca_topic_score_gemma":0.041363623,"teacher_disagreement_score":0.018419145,"about_ca_system_score_codex":0.0002885275,"about_ca_system_score_gemma":0.00013292325,"threshold_uncertainty_score":0.036623895},"labels":[],"label_agreement":null},{"id":"W2066164130","doi":"10.1086/344785","title":"Discovery of the Low‐Redshift Optical Afterglow of GRB 011121 and Its Progenitor Supernova SN 2001ke","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":172,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Gamma-ray burst; Afterglow; Astrophysics; Supernova; Redshift; Photometry (optics); Light curve; Astronomy; Galaxy; Pair-instability supernova; Fermi Gamma-ray Space Telescope; Spectral energy distribution; Stars; Ejecta","score_opus":0.00799043950088451,"score_gpt":0.21426983159007762,"score_spread":0.2062793920891931,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066164130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99889815,0.00016648672,0.00011593542,0.000039388204,0.000009873267,0.0000049773007,0.00017730297,0.000022858885,0.00056494575],"genre_scores_gemma":[0.9970299,0.00015415269,0.0004386889,0.00006129478,0.000027647306,0.000013920327,0.0014227341,0.000009146034,0.00084242923],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998838,0.000010099457,0.0000098255605,0.000044522578,0.000022683918,0.000029205974],"domain_scores_gemma":[0.99936837,0.00007445083,0.00025146359,0.00007477002,0.00007384594,0.00015710997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022401169,0.0003281513,0.0004386435,0.0006968829,0.0004988254,0.0009020099,0.00037758515,0.0007117535,0.0009846644],"category_scores_gemma":[0.00076319335,0.0003040014,0.00028892665,0.0005117381,0.00025948064,0.00041672084,0.0009104967,0.0007610324,0.00042049625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008246221,0.00031824014,0.8707724,0.00021304248,0.00015699647,0.006459503,0.0007529559,0.00035615556,0.09345425,0.0002602461,0.00095451786,0.02547709],"study_design_scores_gemma":[0.000016367916,0.00024584052,0.9895511,0.000017360495,0.00002808057,0.004793217,0.00017916232,0.00022494158,0.0025033455,0.000047487505,0.0023779785,0.0000149701345],"about_ca_topic_score_codex":0.00086424826,"about_ca_topic_score_gemma":0.002096671,"teacher_disagreement_score":0.0009846644,"about_ca_system_score_codex":0.00017170918,"about_ca_system_score_gemma":0.000087977896,"threshold_uncertainty_score":0.0032940507},"labels":[],"label_agreement":null},{"id":"W2066343624","doi":"10.1088/0004-637x/728/2/123","title":"FORMATION OF COLLAPSING CORES IN SUBCRITICAL MAGNETIC CLOUDS: THREE-DIMENSIONAL MAGNETOHYDRODYNAMIC SIMULATIONS WITH AMBIPOLAR DIFFUSION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Physics; Supersonic speed; Magnetic field; Magnetohydrodynamics; Molecular cloud; Mechanics; Magnetohydrodynamic drive; Diffusion; Computational physics; Astrophysics; Plasma","score_opus":0.011727980840153772,"score_gpt":0.21914204024215364,"score_spread":0.20741405940199986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066343624","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993458,0.00008385346,0.0031836932,0.00022158067,0.000018999135,0.000032158496,0.00012771587,0.00004757879,0.0028266127],"genre_scores_gemma":[0.9978454,0.000067735695,0.0014575205,0.000051079634,0.000010347918,0.000036946374,0.00011360451,0.00001991724,0.00039739872],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998709,0.000026744188,0.0000061400797,0.0000147197925,0.000021413292,0.00006002752],"domain_scores_gemma":[0.9993525,0.00028465694,0.000090041045,0.000031773812,0.000062576895,0.00017849836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032980103,0.00047190837,0.00081944116,0.00052375474,0.0008809814,0.0010238186,0.0011035674,0.0012802857,0.0010317159],"category_scores_gemma":[0.0014218945,0.0004566296,0.0007723067,0.0005902194,0.00096798694,0.0006147678,0.00088829023,0.00087527046,0.00010298519],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012524484,0.00010510926,0.0048202546,0.000020725369,0.000043419146,0.0001865552,0.00008940999,0.9902829,0.0018225441,0.0016463948,0.00014197244,0.00071552803],"study_design_scores_gemma":[0.000049055332,0.000021381164,0.0007869641,0.0000026591667,0.0000066917023,0.00000908151,0.00002683198,0.99845254,0.00028328612,0.0002689817,0.0000857562,0.000006723995],"about_ca_topic_score_codex":0.028770747,"about_ca_topic_score_gemma":0.010983026,"teacher_disagreement_score":0.028770747,"about_ca_system_score_codex":0.0012424375,"about_ca_system_score_gemma":0.0010955882,"threshold_uncertainty_score":0.05720657},"labels":[],"label_agreement":null},{"id":"W2066464280","doi":"10.1088/0004-637x/767/1/31","title":"A THERMAL INFRARED IMAGING STUDY OF VERY LOW MASS, WIDE-SEPARATION BROWN DWARF COMPANIONS TO UPPER SCORPIUS STARS: CONSTRAINING CIRCUMSTELLAR ENVIRONMENTS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Photometry (optics); Stars; Circumstellar disk; Infrared; Infrared excess; Thermal; Stellar classification","score_opus":0.010814368044189135,"score_gpt":0.2266907730096631,"score_spread":0.21587640496547394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066464280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943596,0.000043493554,0.000108161476,0.000005231767,4.4294572e-7,0.0000030906601,0.000028737477,0.000009280628,0.00036553168],"genre_scores_gemma":[0.9987368,0.000049934046,0.0007535589,0.000010076497,0.0000044505514,0.000003649629,0.00015457292,0.000005407327,0.00028156114],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993515,0.0000048511865,0.0000035549185,0.000019672805,0.000016181606,0.00002058959],"domain_scores_gemma":[0.99981815,0.00001565248,0.0000613589,0.000014869331,0.000030851606,0.000059112197],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015192883,0.00032234337,0.00017697786,0.001030809,0.00044905362,0.00036407687,0.00023792684,0.00024942248,0.0006512372],"category_scores_gemma":[0.00018551455,0.0002051831,0.00019091635,0.00044499373,0.0002847451,0.00021433443,0.0004361537,0.00020064686,0.00024457255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026139393,0.00014403922,0.5476757,0.00006176703,0.00006922675,0.0023633472,0.0007828036,0.00052090763,0.43480116,0.000103751125,0.0001889016,0.013027012],"study_design_scores_gemma":[0.000004583449,0.000100427045,0.9902457,0.0000036098113,0.00002385661,0.0013935731,0.00032000348,0.00058469694,0.0069723623,0.000023858132,0.00032344935,0.0000039506976],"about_ca_topic_score_codex":0.0037780954,"about_ca_topic_score_gemma":0.008144545,"teacher_disagreement_score":0.0037780954,"about_ca_system_score_codex":0.00029260328,"about_ca_system_score_gemma":0.000158144,"threshold_uncertainty_score":0.007512212},"labels":[],"label_agreement":null},{"id":"W2066869552","doi":"10.1088/0004-637x/741/2/110","title":"THE BOLOCAM GALACTIC PLANE SURVEY. VII. CHARACTERIZING THE PROPERTIES OF MASSIVE STAR-FORMING REGIONS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":142,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"Science and Technology Facilities Council; Canadian Space Agency; Commonwealth Scientific and Industrial Research Organisation; Associated Universities; University of Texas at Austin; National Radio Astronomy Observatory; National Science Foundation","keywords":"Astrophysics; Physics; Galactic plane; Stars; Galaxy; Star formation; Spiral galaxy; Molecular cloud; Astronomy","score_opus":0.03853167650251305,"score_gpt":0.22807525347992993,"score_spread":0.1895435769774169,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066869552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8806342,0.0025590644,0.0013067331,0.0004988118,0.000060486484,0.00014818729,0.097445704,0.0003848374,0.01696194],"genre_scores_gemma":[0.88287467,0.0014857276,0.0041504544,0.00025211534,0.000091700036,0.0001312762,0.105308086,0.00007269298,0.005633346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986684,0.000021610067,0.0000094089655,0.000030115094,0.000038530725,0.00003346592],"domain_scores_gemma":[0.9994048,0.000027462507,0.00025437298,0.000050289942,0.00010982678,0.00015323437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003024271,0.00036047472,0.00017068535,0.0023554685,0.00018991758,0.0005414199,0.0003593224,0.00019360744,0.0018792517],"category_scores_gemma":[0.00056567887,0.00011645346,0.00018034378,0.0018847532,0.00011289583,0.00020673212,0.0005236494,0.00024256356,0.0010721581],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013156256,0.000020829522,0.96749103,0.000058852387,0.00007899126,0.000098367454,0.00018129178,0.00013216541,0.0034144474,0.00021022896,0.009405384,0.01877691],"study_design_scores_gemma":[0.0000101789965,0.000011492393,0.9935322,0.000012840354,0.000010641708,0.000045887577,0.000057145822,0.00008439237,0.00028031276,0.00002478962,0.005928686,0.0000014905465],"about_ca_topic_score_codex":0.058559787,"about_ca_topic_score_gemma":0.071801305,"teacher_disagreement_score":0.058559787,"about_ca_system_score_codex":0.0007494043,"about_ca_system_score_gemma":0.00030917407,"threshold_uncertainty_score":0.11643785},"labels":[],"label_agreement":null},{"id":"W2066870943","doi":"10.1086/342225","title":"Gravitational Microlensing Events Due to Stellar‐Mass Black Holes","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gravitational microlensing; Physics; Astrophysics; Bulge; Astronomy; Galaxy; Black hole (networking); Stars; Parallax","score_opus":0.014836898131477911,"score_gpt":0.22702449907903238,"score_spread":0.21218760094755448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066870943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994467,0.000094314244,0.000050338214,0.000010673539,0.0000015538166,0.000003440422,0.0001600395,0.0000104384735,0.00022248994],"genre_scores_gemma":[0.99911433,0.000048911817,0.00011791149,0.000009024828,0.000013598678,0.0000031314444,0.0005780535,0.0000020196155,0.00011302675],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955016,0.000042437827,0.00003729749,0.00007882336,0.00012302543,0.00016824102],"domain_scores_gemma":[0.99761957,0.00038793695,0.0011739486,0.00013917148,0.00014718487,0.00053218164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030121394,0.0002679042,0.00028686557,0.0025076987,0.0005578825,0.00070204027,0.00033944641,0.00035387857,0.0011045228],"category_scores_gemma":[0.0014214829,0.0001656248,0.00034743888,0.0012148266,0.00030968204,0.00034880606,0.0011269781,0.00021377989,0.00019562525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002269734,0.000041103667,0.9861058,0.000019154488,0.00007370328,0.0011291866,0.00031493028,0.00020529717,0.0037773093,0.00011171036,0.00025978737,0.007734992],"study_design_scores_gemma":[0.0000065173863,0.000053096024,0.996876,0.0000034440216,0.000020676687,0.0010928427,0.00013338299,0.00043679302,0.00092168554,0.000053266074,0.00039438557,0.000007857601],"about_ca_topic_score_codex":0.00432966,"about_ca_topic_score_gemma":0.0066881385,"teacher_disagreement_score":0.00432966,"about_ca_system_score_codex":0.00037074252,"about_ca_system_score_gemma":0.00015570523,"threshold_uncertainty_score":0.008608878},"labels":[],"label_agreement":null},{"id":"W2066895865","doi":"10.1086/381730","title":"Green Bank Telescope Discovery of Two Binary Millisecond Pulsars in the Globular Cluster M30","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Steacie Institute for Molecular Sciences; Research Canada; University of British Columbia; McGill University","funders":"","keywords":"Physics; Pulsar; Millisecond pulsar; Astrophysics; Neutron star; Globular cluster; Green Bank Telescope; Astronomy; Binary pulsar; Eclipse; Orbital eccentricity; X-ray pulsar; Galaxy; Stars","score_opus":0.009470382137791252,"score_gpt":0.23357211527426947,"score_spread":0.22410173313647822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066895865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99847,0.00011373103,0.00011599674,0.000083697494,0.000008193,0.000009113928,0.00015387457,0.000014139896,0.0010312597],"genre_scores_gemma":[0.99822706,0.00009099427,0.0005368665,0.0001029856,0.000008730748,0.00001055641,0.00036087638,0.0000060521124,0.00065587135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989986,0.00000634404,0.000004028612,0.000026083493,0.000031634132,0.000032098727],"domain_scores_gemma":[0.99967766,0.000019743042,0.000065989945,0.000021463042,0.000028965202,0.00018621761],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023041443,0.00018419579,0.00015918382,0.00071420055,0.0007204102,0.00044589795,0.00033741925,0.0004368211,0.0006760877],"category_scores_gemma":[0.00038214124,0.00021522546,0.00019442067,0.0003389967,0.0003514582,0.00021264511,0.001366667,0.0003590591,0.00040268866],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009044582,0.0001422517,0.7496754,0.000072187686,0.00007559197,0.005359103,0.0032821426,0.00039984184,0.21464889,0.001769637,0.0022985404,0.021372011],"study_design_scores_gemma":[0.00003351657,0.00021373856,0.9876281,0.000015510983,0.000016636794,0.0020917407,0.00035531283,0.0007150403,0.005166548,0.0003578748,0.0033851203,0.00002091934],"about_ca_topic_score_codex":0.010475692,"about_ca_topic_score_gemma":0.019690035,"teacher_disagreement_score":0.010475692,"about_ca_system_score_codex":0.0005797054,"about_ca_system_score_gemma":0.0004160306,"threshold_uncertainty_score":0.02082944},"labels":[],"label_agreement":null},{"id":"W2066928321","doi":"10.1088/0004-637x/695/2/1537","title":"LUMINOUS INFRARED GALAXIES WITH THE SUBMILLIMETER ARRAY. II. COMPARING THE CO (3-2) SIZES AND LUMINOSITIES OF LOCAL AND HIGH-REDSHIFT LUMINOUS INFRARED GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Luminous infrared galaxy; Star formation; Halo; Infrared; Population; Line (geometry); Luminosity","score_opus":0.006535250601717829,"score_gpt":0.19514588705037136,"score_spread":0.18861063644865353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066928321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9679478,0.002733516,0.011136802,0.0002644144,0.00006552972,0.00007638803,0.0043687625,0.00045853585,0.012948358],"genre_scores_gemma":[0.9764483,0.0006065296,0.016752793,0.0003591376,0.0001275771,0.000095288495,0.003508177,0.00003524118,0.002066932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996414,0.000062650695,0.000016292879,0.00013897239,0.00007639186,0.00006428491],"domain_scores_gemma":[0.9990006,0.00011279057,0.0005327847,0.00015614534,0.000088292734,0.00010935614],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005542353,0.00025940692,0.00019278402,0.0012720192,0.00015729491,0.00062991166,0.0004226507,0.00038742015,0.0027722637],"category_scores_gemma":[0.00076436123,0.00014872271,0.00042218462,0.0014684526,0.00018682922,0.00072847726,0.0005936705,0.0003571027,0.0009959813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000119053366,0.00004832422,0.94421893,0.00006444382,0.00013968468,0.00006519401,0.00010266066,0.00038270993,0.014062836,0.000736174,0.0009936772,0.039066322],"study_design_scores_gemma":[0.0000039553206,0.00005223033,0.99567395,0.000008207371,0.00002046327,0.0001279916,0.00004386284,0.00045016964,0.0013094627,0.0001741388,0.0021317077,0.0000037936184],"about_ca_topic_score_codex":0.0015536014,"about_ca_topic_score_gemma":0.006034918,"teacher_disagreement_score":0.0027722637,"about_ca_system_score_codex":0.00023212754,"about_ca_system_score_gemma":0.000101977275,"threshold_uncertainty_score":0.009274185},"labels":[],"label_agreement":null},{"id":"W2066948687","doi":"10.1088/0004-637x/755/2/165","title":"SPATIALLY RESOLVED STELLAR, DUST, AND GAS PROPERTIES OF THE POST-INTERACTING WHIRLPOOL GALAXY SYSTEM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Spiral galaxy; Stellar mass; Star formation; Milky Way; Astronomy; Dust lane; Mass ratio; Infrared","score_opus":0.01012411024339543,"score_gpt":0.19736284409382113,"score_spread":0.1872387338504257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2066948687","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999775,0.000018571263,0.000024135094,0.0000035609585,1.9740105e-7,8.8100825e-7,0.000040994102,0.0000072797648,0.00012940564],"genre_scores_gemma":[0.9996623,0.00001352386,0.00009218528,0.000004236282,7.9765545e-7,0.0000014627038,0.00014090049,0.000002069247,0.000082503466],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987507,0.000007778672,0.000007341851,0.00005007574,0.000020290572,0.00003937867],"domain_scores_gemma":[0.99961543,0.00003746091,0.00018265516,0.00005091279,0.000035529913,0.00007799636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012661346,0.00020175398,0.00026369197,0.0008914286,0.0004259575,0.0005969486,0.00033477548,0.00021248683,0.00094870443],"category_scores_gemma":[0.00037199314,0.000202596,0.00030394434,0.0005177692,0.0002849531,0.00029220936,0.0006900964,0.00018792802,0.00016885663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021568642,0.000036355283,0.9269352,0.000026352449,0.00012743265,0.0005775653,0.0007962848,0.00086728326,0.06330757,0.00012839379,0.00014289486,0.0068390574],"study_design_scores_gemma":[0.000002024515,0.000014352656,0.99866724,0.0000014727354,0.000012176828,0.000073908595,0.00008590553,0.00034212568,0.0007039751,0.000011776553,0.00008172942,0.0000031288555],"about_ca_topic_score_codex":0.01902468,"about_ca_topic_score_gemma":0.027959965,"teacher_disagreement_score":0.01902468,"about_ca_system_score_codex":0.00071009016,"about_ca_system_score_gemma":0.0001730834,"threshold_uncertainty_score":0.03782785},"labels":[],"label_agreement":null},{"id":"W2067111130","doi":"10.1086/321591","title":"Gaussianity of Degree‐Scale Cosmic Microwave Background Anisotropy Observations","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Cosmic microwave background; Anisotropy; Physics; Astrophysics; Non-Gaussianity; Cold dark matter; Gaussian; Degree (music); Scale (ratio); Cosmology; Optics; Quantum mechanics","score_opus":0.03351851433370293,"score_gpt":0.26584553040810793,"score_spread":0.232327016074405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067111130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951315,0.000035791836,0.0034184877,0.000034219906,0.0000012826683,0.000005006333,0.00022360325,0.00006781437,0.0010822031],"genre_scores_gemma":[0.9993068,0.000010422521,0.00038825665,0.0000042562588,0.0000017152453,0.0000018889629,0.00022921873,0.000010413926,0.000047178113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999313,0.0002008011,0.000033225857,0.0001589851,0.00016928172,0.0001247121],"domain_scores_gemma":[0.99348915,0.0026674217,0.0012749098,0.0015868688,0.00062765885,0.00035390156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014117567,0.0002816047,0.00025628728,0.0007538904,0.0003149525,0.00083968556,0.0002546063,0.00019871723,0.00060893164],"category_scores_gemma":[0.007654189,0.00025176725,0.00030529682,0.0009826088,0.0009795845,0.00060558633,0.00074826716,0.00034748693,0.00008505856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008450053,0.000049146758,0.88893807,0.00005591244,0.0003187276,0.00027676008,0.0005695092,0.042755947,0.043735243,0.007941578,0.00048687484,0.0140273515],"study_design_scores_gemma":[0.00002764076,0.000078806785,0.93671113,0.000008424242,0.00005527222,0.00021153827,0.0001639201,0.049623594,0.0075793355,0.0049235225,0.00057654275,0.000040302577],"about_ca_topic_score_codex":0.0096203005,"about_ca_topic_score_gemma":0.008968511,"teacher_disagreement_score":0.0096203005,"about_ca_system_score_codex":0.0006698839,"about_ca_system_score_gemma":0.00031905575,"threshold_uncertainty_score":0.01912862},"labels":[],"label_agreement":null},{"id":"W2067205827","doi":"10.1088/0004-637x/776/2/69","title":"DISCOVERY OF A NEW TeV GAMMA-RAY SOURCE: VER J0521+211","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Blazar; Crab Nebula; Astrophysics; Cherenkov radiation; Fermi Gamma-ray Space Telescope; Cherenkov Telescope Array; Flux (metallurgy); Gamma ray; Photon; BL Lac object; Redshift; Astronomy; Telescope; Photon flux; Galaxy; Detector; Optics","score_opus":0.0069897473574849385,"score_gpt":0.20570803209770738,"score_spread":0.19871828474022243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067205827","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953483,0.00045406047,0.00040423896,0.00011960089,0.000048439168,0.00001719334,0.00023089517,0.000052113206,0.003325228],"genre_scores_gemma":[0.9963654,0.00025740932,0.0010394519,0.0001699873,0.00010830698,0.000014576374,0.0011397448,0.00001424037,0.0008908307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972945,0.000017956427,0.000021087497,0.00008366515,0.0000869586,0.000060794835],"domain_scores_gemma":[0.9993917,0.00008542535,0.000184457,0.00009432299,0.00006092523,0.00018327919],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037579454,0.00034284228,0.00050839345,0.0008874933,0.001259501,0.0019227352,0.00054800237,0.00097252487,0.001348031],"category_scores_gemma":[0.00060634926,0.00038536917,0.0004269329,0.0009820327,0.0005753244,0.0005613533,0.0011588499,0.0006813273,0.0004965769],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009435107,0.00036472178,0.72122395,0.0002427739,0.00027945955,0.024037968,0.0010816959,0.0012322492,0.21743359,0.0024317245,0.00357757,0.027150773],"study_design_scores_gemma":[0.00006842025,0.00052290526,0.9528674,0.00004118086,0.0001422408,0.016557727,0.00025926798,0.0017203417,0.010690319,0.0005135967,0.016565947,0.000050750856],"about_ca_topic_score_codex":0.0010591344,"about_ca_topic_score_gemma":0.002243213,"teacher_disagreement_score":0.0019227352,"about_ca_system_score_codex":0.0005242459,"about_ca_system_score_gemma":0.00027658767,"threshold_uncertainty_score":0.004509568},"labels":[],"label_agreement":null},{"id":"W2067217178","doi":"10.1086/321695","title":"Discovery of Two New Pulsating DA (ZZ Ceti) White Dwarfs","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Instability strip; Physics; White dwarf; Astrophysics; Luminosity; Light curve; Amplitude; Stars; Spectral line; Effective temperature; Astronomy; Cepheid variable; Optics","score_opus":0.015567174815656858,"score_gpt":0.24832277392498298,"score_spread":0.2327555991093261,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067217178","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992093,0.000064230226,0.00017954863,0.00001588488,0.0000043974173,0.0000041552316,0.00008466989,0.000007997252,0.00042974442],"genre_scores_gemma":[0.99876726,0.00004522701,0.00056760845,0.000018869467,0.000009883966,0.0000052628184,0.00031707168,0.0000034552545,0.00026536605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989307,0.000006009372,0.000011644185,0.000040778432,0.000029246885,0.00001923208],"domain_scores_gemma":[0.9996222,0.000026392563,0.00016369358,0.00003513139,0.00002880191,0.00012360788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013365876,0.00016150021,0.00019679265,0.00075922185,0.00035254264,0.00055510044,0.00028766558,0.00026709697,0.0005508145],"category_scores_gemma":[0.00043868535,0.00012641792,0.00010361512,0.00048121877,0.00032601994,0.00019631027,0.00072651694,0.00024028635,0.00018374357],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021642882,0.000044692395,0.8731392,0.000046345318,0.00002870993,0.0012546689,0.0006663782,0.00009642801,0.110053755,0.0006511176,0.00018958552,0.013612738],"study_design_scores_gemma":[0.000009468271,0.00017932538,0.98443526,0.0000047151684,0.000017613158,0.00321788,0.00026613864,0.00029274356,0.007775938,0.00020757182,0.0035855107,0.0000078533885],"about_ca_topic_score_codex":0.00047077305,"about_ca_topic_score_gemma":0.0008573197,"teacher_disagreement_score":0.00075922185,"about_ca_system_score_codex":0.00022433166,"about_ca_system_score_gemma":0.00010044487,"threshold_uncertainty_score":0.001842618},"labels":[],"label_agreement":null},{"id":"W2067295692","doi":"10.1086/506957","title":"Silicon and Carbon Isotopic Ratios in AGB Stars: SiC Grain Data, Models, and the Galactic Evolution of the Si Isotopes","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":147,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Nucleosynthesis; Astrophysics; Metallicity; Asymptotic giant branch; Stellar nucleosynthesis; Galaxy; Stars; Isotope; Nuclear physics","score_opus":0.00911350493415267,"score_gpt":0.20227177487004,"score_spread":0.19315826993588733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067295692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99836427,0.000092689035,0.00036475237,0.00003236006,0.0000015340012,0.0000030698009,0.0004128734,0.000023915582,0.0007045895],"genre_scores_gemma":[0.9987489,0.000043244807,0.0003052227,0.000008411722,0.0000017185961,0.0000032399694,0.00074725103,0.0000146593675,0.00012737319],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983585,0.000035358506,0.00001143877,0.000057151214,0.0000372497,0.000022821852],"domain_scores_gemma":[0.99936587,0.0002646913,0.000097527,0.000086747765,0.00010406495,0.00008102469],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009926382,0.0006480421,0.0004776232,0.00095838815,0.0004310914,0.000933848,0.0012670676,0.0008533733,0.0012411908],"category_scores_gemma":[0.0015446123,0.00036409075,0.0006285201,0.0010533455,0.0005122884,0.00066156563,0.00033406098,0.00028008677,0.0003848013],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018888026,0.0001908154,0.71620995,0.00013907599,0.00029941738,0.00018311956,0.00029175373,0.24911927,0.015109349,0.0041027754,0.000794489,0.011671267],"study_design_scores_gemma":[0.00036244863,0.00029844433,0.39394704,0.000026824702,0.000198933,0.00025452243,0.00019543873,0.58758307,0.010801267,0.0045153596,0.0017639268,0.000052672203],"about_ca_topic_score_codex":0.04351788,"about_ca_topic_score_gemma":0.028215135,"teacher_disagreement_score":0.04351788,"about_ca_system_score_codex":0.0027284694,"about_ca_system_score_gemma":0.0005182474,"threshold_uncertainty_score":0.086529195},"labels":[],"label_agreement":null},{"id":"W2067351366","doi":"10.1088/0004-637x/769/1/11","title":"LINE EMISSION FROM RADIATION-PRESSURIZED H II REGIONS. I. INTERNAL STRUCTURE AND LINE RATIOS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Ionization; Line (geometry); Emission spectrum; Stars; Population; Luminosity; Radiation pressure; Radiation","score_opus":0.005423198135954894,"score_gpt":0.20708378307038644,"score_spread":0.20166058493443154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067351366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898129,0.000050818224,0.00693596,0.000023973626,0.0000019988224,0.000007666823,0.00066733494,0.000117516036,0.0023818603],"genre_scores_gemma":[0.99754804,0.000021520735,0.001726013,0.0000050212907,9.495022e-7,0.0000040927,0.0004441199,0.0000192436,0.00023111411],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999565,0.000008151211,0.0000018036603,0.000015565845,0.000008176078,0.000009791291],"domain_scores_gemma":[0.9996829,0.00009728256,0.00010745198,0.00004479765,0.000029153081,0.000038313327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015013888,0.00025296648,0.00012552003,0.00027000945,0.00014092702,0.0004688509,0.0005235957,0.00020643251,0.0012948266],"category_scores_gemma":[0.00070381106,0.00021447732,0.00030130643,0.0003120572,0.000272815,0.00039174478,0.00033182578,0.00018903145,0.00021176822],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017869065,0.00007394873,0.3982757,0.0000421645,0.00008852057,0.00018785094,0.00013559757,0.56086886,0.024593307,0.005436443,0.000490809,0.009628201],"study_design_scores_gemma":[0.000035452424,0.00008664157,0.21700418,0.000008421211,0.000044261975,0.00022298185,0.000116364376,0.7659727,0.011540604,0.0041869907,0.0007591323,0.000022243927],"about_ca_topic_score_codex":0.0051158452,"about_ca_topic_score_gemma":0.0037997533,"teacher_disagreement_score":0.0051158452,"about_ca_system_score_codex":0.0004675468,"about_ca_system_score_gemma":0.000089181565,"threshold_uncertainty_score":0.010172129},"labels":[],"label_agreement":null},{"id":"W2067356016","doi":"10.1088/0004-637x/745/1/14","title":"PROBING THE FLARE ATMOSPHERES OF M DWARFS USING INFRARED EMISSION LINES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Flare; Infrared; Emission spectrum; Spectroscopy; Photometry (optics); Radiative transfer; Chromosphere; Spectral line; Infrared spectroscopy; Line (geometry); Astronomy; Stars; Optics","score_opus":0.027142060118405257,"score_gpt":0.23736184831737145,"score_spread":0.2102197881989662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067356016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99851865,0.000033952696,0.000718851,0.000010640416,0.0000015575255,0.0000055295272,0.00016521862,0.00007852476,0.00046705094],"genre_scores_gemma":[0.9982951,0.000030375162,0.0011531657,0.000012707641,0.0000043077935,0.000004627489,0.00039399715,0.000019606554,0.00008599474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992764,0.000012086568,0.0000025011027,0.000023570072,0.000015728267,0.00001849708],"domain_scores_gemma":[0.99984455,0.000038565966,0.000038905528,0.000019786848,0.000017015525,0.000041230604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024566677,0.00029675613,0.00018054181,0.0003142303,0.00032144177,0.0002770519,0.0003372901,0.0002388346,0.0002895954],"category_scores_gemma":[0.00034292185,0.00017739093,0.00033889865,0.00024191779,0.00015485725,0.00022839777,0.00027122934,0.00025656793,0.00007985899],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033772693,0.0002562012,0.8499558,0.000052368894,0.00020296873,0.0002306122,0.00052630116,0.039937414,0.092785284,0.00048810893,0.00045365127,0.014773664],"study_design_scores_gemma":[0.000060699174,0.00023623754,0.8700646,0.0000063458915,0.00008657752,0.0001090552,0.00015577252,0.11771571,0.010027665,0.00034065862,0.0011663135,0.00003032388],"about_ca_topic_score_codex":0.014457434,"about_ca_topic_score_gemma":0.019584257,"teacher_disagreement_score":0.014457434,"about_ca_system_score_codex":0.0005326434,"about_ca_system_score_gemma":0.00014203244,"threshold_uncertainty_score":0.028746545},"labels":[],"label_agreement":null},{"id":"W2067437743","doi":"10.1086/498224","title":"Composition of the Innermost Core‐Collapse Supernova Ejecta","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":225,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Neutrino; Supernova; Ejecta; Nucleosynthesis; Astrophysics; Stars; Neutron star; Nuclear physics","score_opus":0.013847688331052325,"score_gpt":0.26065671474042273,"score_spread":0.2468090264093704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067437743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937358,0.0002442719,0.0017910729,0.000019524494,0.000008673573,0.000008458496,0.0013377016,0.00013112507,0.0027233043],"genre_scores_gemma":[0.9940055,0.00018843666,0.0013103008,0.000022211767,0.000003903061,0.00001292819,0.002957619,0.00009417158,0.0014048817],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999373,0.000005481134,0.0000041549015,0.000023632285,0.000012630405,0.000016744285],"domain_scores_gemma":[0.9998536,0.000019907182,0.00004099463,0.00001193756,0.000035878606,0.000037700604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108655746,0.00039281542,0.00018088437,0.0011132684,0.00022546062,0.0005980891,0.00023346952,0.00031622974,0.002134574],"category_scores_gemma":[0.0002776302,0.0002312014,0.00036328347,0.00036451014,0.00012954866,0.0001754519,0.0002727076,0.00022395766,0.0004883915],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009408554,0.0001791571,0.15053067,0.00014812317,0.0002866635,0.0007235554,0.00020852132,0.06290514,0.76443,0.0016561693,0.0006941993,0.017296933],"study_design_scores_gemma":[0.000064857224,0.00026086834,0.62851,0.00003581988,0.0001749444,0.0006766398,0.000209785,0.14277463,0.2211728,0.0007579288,0.0052945223,0.00006727241],"about_ca_topic_score_codex":0.0037002813,"about_ca_topic_score_gemma":0.0017183756,"teacher_disagreement_score":0.0037002813,"about_ca_system_score_codex":0.00029025134,"about_ca_system_score_gemma":0.00018959626,"threshold_uncertainty_score":0.007357478},"labels":[],"label_agreement":null},{"id":"W2067439679","doi":"10.1086/320692","title":"The Detection of Bright Asymptotic Giant Branch Stars in the Nearby Elliptical Galaxy Maffei 1","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Distance modulus; Astrophysics; Surface brightness; Galaxy; Asymptotic giant branch; Luminosity; Bulge; Surface brightness fluctuation; Elliptical galaxy; Stars; Luminosity function; Globular cluster; Galaxy group","score_opus":0.008312811680450293,"score_gpt":0.21528676776700978,"score_spread":0.2069739560865595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067439679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992673,0.00007666397,0.00008053893,0.00001624572,0.000002222869,0.0000015756474,0.000017620625,0.00000481915,0.00053292414],"genre_scores_gemma":[0.9992505,0.000043385193,0.00034365238,0.000012886748,0.000006109066,0.0000021265905,0.0000823952,0.000001562307,0.00025744093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984944,0.000022086357,0.0000063414154,0.000044526147,0.000029336394,0.000048298854],"domain_scores_gemma":[0.999597,0.00007773236,0.00009310125,0.000050318664,0.00007041579,0.000111487985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000403859,0.00019030097,0.00018365074,0.001053501,0.0005401606,0.00047898619,0.000324815,0.00039540854,0.00080254197],"category_scores_gemma":[0.00092830876,0.00018472994,0.00015521767,0.00023797879,0.00038439393,0.0003732325,0.00062991737,0.00025087778,0.00017986381],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001499135,0.00008492955,0.8804754,0.000032427404,0.00003865059,0.0006176479,0.0010641271,0.00018721056,0.10054643,0.00041340053,0.00027034298,0.016119473],"study_design_scores_gemma":[0.0000048271777,0.00013394929,0.99371755,0.00000737744,0.000013476928,0.0008925644,0.00016456038,0.00024525667,0.0038447944,0.00008429468,0.0008848008,0.0000065365675],"about_ca_topic_score_codex":0.002120517,"about_ca_topic_score_gemma":0.0045725727,"teacher_disagreement_score":0.002120517,"about_ca_system_score_codex":0.00031950074,"about_ca_system_score_gemma":0.000089554655,"threshold_uncertainty_score":0.0042163134},"labels":[],"label_agreement":null},{"id":"W2067526604","doi":"10.1088/0004-637x/725/2/1971","title":"A SIMPLE CONNECTION BETWEEN THE NEAR- AND MID-INFRARED EMISSION OF GALAXIES AND THEIR STAR FORMATION RATES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Star formation; Galaxy; Extinction (optical mineralogy); Spectral energy distribution; Luminous infrared galaxy; Infrared; Wavelength; Dust lane","score_opus":0.010118974266770237,"score_gpt":0.23970143918432116,"score_spread":0.2295824649175509,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067526604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931335,0.00045052878,0.0026492004,0.000072512565,0.0000060734005,0.000025972244,0.00057059975,0.00006673587,0.0030250358],"genre_scores_gemma":[0.9978613,0.000079503865,0.0010511084,0.000025312062,0.00000879964,0.000011372823,0.00026903994,0.000008824904,0.00068472757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996742,0.0000731666,0.000026944375,0.00010988394,0.000055942663,0.000059898095],"domain_scores_gemma":[0.99622643,0.0015309274,0.0011105385,0.0004216005,0.00044440752,0.00026618477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053328526,0.0002919824,0.00016695258,0.00080421777,0.00014411371,0.0005697357,0.00031761112,0.00041974374,0.002485339],"category_scores_gemma":[0.003957243,0.00023808976,0.00017912016,0.0005260459,0.00045390922,0.0007506766,0.00033712102,0.00041106791,0.0008079862],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006791994,0.000033823195,0.9853591,0.000025904372,0.000050920786,0.000029477296,0.00011550595,0.0004985978,0.008614065,0.00038292125,0.00006912426,0.004752837],"study_design_scores_gemma":[0.0000032047274,0.000046678808,0.9973354,0.0000043745486,0.000013052033,0.00009515604,0.000045627334,0.00068607647,0.0012807216,0.0002586607,0.00022620894,0.000004783471],"about_ca_topic_score_codex":0.0012428387,"about_ca_topic_score_gemma":0.0013603935,"teacher_disagreement_score":0.002485339,"about_ca_system_score_codex":0.00016957075,"about_ca_system_score_gemma":0.000092356546,"threshold_uncertainty_score":0.008314252},"labels":[],"label_agreement":null},{"id":"W2067614322","doi":"10.1086/342142","title":"The Quadruple Wolf‐Rayet System GP Cephei: Spectral Types, Masses, Mass‐Loss Rate, and Colliding Winds","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; Astrophysics; Wolf–Rayet star; Orbital period; Astronomy; Stars","score_opus":0.010655363890269724,"score_gpt":0.21363070151181918,"score_spread":0.20297533762154946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067614322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99857366,0.00007669285,0.00014067968,0.000025901358,0.0000037979562,0.000003982153,0.00028117388,0.00001566383,0.00087842083],"genre_scores_gemma":[0.9991379,0.00002058933,0.00009252381,0.000009947334,0.0000040320583,0.0000018481193,0.00028860813,0.0000069936186,0.00043746608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.000010935452,0.0000033840058,0.00002134047,0.000015821472,0.000019594194],"domain_scores_gemma":[0.99937963,0.00014539415,0.00017255332,0.00006722544,0.000071010036,0.0001641982],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019238298,0.000255395,0.00032394534,0.00071234896,0.00054939487,0.0006101095,0.0002576463,0.0003272291,0.0033742546],"category_scores_gemma":[0.00070812536,0.00017963449,0.00006306294,0.0005303983,0.00018678789,0.00036498945,0.00038245192,0.00026015544,0.0007801541],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008946225,0.00009416167,0.9090684,0.00006396753,0.000086502514,0.0019521955,0.0007201472,0.0019182097,0.05818592,0.0010850145,0.002793534,0.023137283],"study_design_scores_gemma":[0.000023156104,0.00011625862,0.9911389,0.000005774502,0.000028808205,0.0009352366,0.00016627711,0.0030840286,0.0023698094,0.00049709564,0.0016191116,0.000015545133],"about_ca_topic_score_codex":0.0018965283,"about_ca_topic_score_gemma":0.003303058,"teacher_disagreement_score":0.0033742546,"about_ca_system_score_codex":0.00011465205,"about_ca_system_score_gemma":0.00012826906,"threshold_uncertainty_score":0.011287987},"labels":[],"label_agreement":null},{"id":"W2067634454","doi":"10.1086/497355","title":"Origin of Tidal Dissipation in Jupiter. II. The Value of<i>Q</i>","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Dissipation; Classification of discontinuities; Tidal acceleration; Turbulence; Tidal force; Jump; Tidal heating; Resonance (particle physics)","score_opus":0.0074406844267152225,"score_gpt":0.23178051459357432,"score_spread":0.2243398301668591,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067634454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98832685,0.000637201,0.0070310566,0.00018157647,0.000013984485,0.000012091776,0.00007228656,0.00017229868,0.0035526038],"genre_scores_gemma":[0.9991986,0.000055537603,0.00045571855,0.000010206461,0.0000040129225,0.0000037898087,0.000025689353,0.000017396813,0.00022899488],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999589,0.0000039520137,0.0000022017698,0.000013168267,0.000008322184,0.000013569386],"domain_scores_gemma":[0.9998857,0.000021508493,0.000046436908,0.000013834792,0.000013613707,0.000018889192],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010841999,0.00022753551,0.00020386734,0.00032466298,0.00038824353,0.0005370363,0.00037241218,0.00029397817,0.00073038193],"category_scores_gemma":[0.0006098185,0.0002094517,0.0001516278,0.00019706115,0.0005094976,0.00044594536,0.00038655652,0.00031212324,0.00015955415],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081959314,0.00013244514,0.19747275,0.00038883789,0.00014198617,0.0026570335,0.002767697,0.10702391,0.5572915,0.06560329,0.0020215525,0.063679464],"study_design_scores_gemma":[0.00007389005,0.0004861805,0.43231174,0.00007915144,0.000078086334,0.0013165312,0.00058396795,0.46951172,0.05502489,0.03409943,0.0063170693,0.00011743899],"about_ca_topic_score_codex":0.0019460707,"about_ca_topic_score_gemma":0.00069785217,"teacher_disagreement_score":0.0019460707,"about_ca_system_score_codex":0.00058761355,"about_ca_system_score_gemma":0.00008638837,"threshold_uncertainty_score":0.0042634606},"labels":[],"label_agreement":null},{"id":"W2067645025","doi":"10.1088/0004-637x/744/2/157","title":"THE ACS LCID PROJECT. VII. THE BLUE STRAGGLERS POPULATION IN THE ISOLATED dSph GALAXIES CETUS AND TUCANA","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Metallicity; Globular cluster; Advanced Camera for Surveys; Photometry (optics); Local Group; Population; Hubble space telescope; Blue straggler; Stars; Dwarf galaxy","score_opus":0.01333790079799287,"score_gpt":0.21775073905534734,"score_spread":0.20441283825735446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067645025","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.005205537,0.0016141937,0.005021118,0.0028267165,0.0009937941,0.00029551698,0.8819543,0.029867627,0.07222123],"genre_scores_gemma":[0.017872598,0.00091754866,0.014469117,0.00080122607,0.00039703114,0.0004349041,0.9268828,0.004073161,0.0341517],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9988883,0.000051783394,0.00003837484,0.00017892287,0.0005792868,0.00026335448],"domain_scores_gemma":[0.9977235,0.00010010591,0.00018168653,0.00039060027,0.0009050395,0.0006990889],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018638088,0.00120456,0.001554652,0.0047580125,0.0018795658,0.0058795884,0.004439357,0.0012898963,0.14685415],"category_scores_gemma":[0.0029530465,0.00056901993,0.00071685755,0.0066696513,0.00037006225,0.0024406477,0.0038811793,0.0014956546,0.091068655],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022563842,0.00006060063,0.0030986285,0.00017946163,0.000051059953,0.00008713549,0.00009264731,0.00027666448,0.0008837232,0.003305577,0.94840693,0.043332],"study_design_scores_gemma":[0.00020622555,0.000014345571,0.009651513,0.00013456761,0.00005932378,0.00007263956,0.00015015824,0.0029822774,0.0014909183,0.0053301333,0.9798672,0.000040748146],"about_ca_topic_score_codex":0.1251471,"about_ca_topic_score_gemma":0.11840735,"teacher_disagreement_score":0.14685415,"about_ca_system_score_codex":0.0031735124,"about_ca_system_score_gemma":0.003936095,"threshold_uncertainty_score":0.4912761},"labels":[],"label_agreement":null},{"id":"W2067722688","doi":"10.1086/526411","title":"Orbital Parameters and Chemical Composition of Four White Dwarfs in Post–Common‐Envelope Binaries","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency","funders":"","keywords":"White dwarf; Astrophysics; Physics; Common envelope; Radial velocity; Low Mass; Spectral line; Astronomy; Stars","score_opus":0.013112533157666969,"score_gpt":0.21102268761410936,"score_spread":0.1979101544564424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067722688","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99970955,0.000025759862,0.000039505816,0.000002312108,5.966326e-7,7.1089784e-7,0.000045500456,0.0000029635694,0.00017316148],"genre_scores_gemma":[0.9995628,0.000011691504,0.000060776238,0.000003857847,0.0000010825993,9.540721e-7,0.0002425443,0.0000027591936,0.00011349342],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990904,0.000006358023,0.0000071250697,0.000029494033,0.0000235637,0.000024385161],"domain_scores_gemma":[0.99978155,0.000027123831,0.00007199143,0.000016063259,0.000027126005,0.000076073564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014482703,0.00020527645,0.00022363289,0.0008026467,0.00036771555,0.00044602784,0.00020362064,0.00029112876,0.0005893585],"category_scores_gemma":[0.00038853215,0.00014222936,0.00014345412,0.0005029303,0.00022066274,0.00029135615,0.00038017237,0.00014140866,0.00016917622],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033305548,0.00006417293,0.953026,0.000009348329,0.00004455816,0.00022778504,0.00027470043,0.0006249956,0.03848822,0.00011646321,0.00008556566,0.006705195],"study_design_scores_gemma":[0.000003138881,0.000029701258,0.9970452,0.0000010275071,0.0000074262566,0.00016534165,0.00009575613,0.0006445979,0.0017930217,0.000042653926,0.00016885293,0.0000032264384],"about_ca_topic_score_codex":0.0040168236,"about_ca_topic_score_gemma":0.0069083674,"teacher_disagreement_score":0.0040168236,"about_ca_system_score_codex":0.0004259047,"about_ca_system_score_gemma":0.00007630966,"threshold_uncertainty_score":0.007986844},"labels":[],"label_agreement":null},{"id":"W2067756552","doi":"10.1088/0004-637x/793/2/75","title":"STRONG BRIGHTNESS VARIATIONS SIGNAL CLOUDY-TO-CLEAR TRANSITION OF BROWN DWARFS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":205,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; York University; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Brown dwarf; Brightness; Photosphere; Amplitude; Telescope; Astronomy; Observatory; Green Bank Telescope; Spectral line; Stars; Galaxy","score_opus":0.00917143927029438,"score_gpt":0.2165146703379123,"score_spread":0.20734323106761793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067756552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881375,0.00002097428,0.00016628511,0.000006567064,0.0000014843765,0.0000019012135,0.00027330808,0.000019493098,0.00069635455],"genre_scores_gemma":[0.9991806,0.000012455598,0.0001761699,0.0000073836827,0.0000040685404,0.000001737497,0.00037029857,0.000005089906,0.00024211954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999471,0.0000039381516,0.000003238419,0.000015884018,0.0000104508645,0.000019394894],"domain_scores_gemma":[0.99976474,0.00004548857,0.00008294317,0.000022091772,0.000026581673,0.000058183425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012425154,0.00010645709,0.000105795145,0.000813769,0.00025340292,0.000300246,0.00014975584,0.00012245767,0.0023821478],"category_scores_gemma":[0.00027232515,0.000060109065,0.00009503635,0.00047717022,0.00027312365,0.000100953606,0.00026035096,0.000090752794,0.0002660689],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038215547,0.000032005846,0.89689386,0.000028359342,0.00003859589,0.0003781386,0.00019910566,0.0002105363,0.09124074,0.00024337097,0.0006670613,0.009686051],"study_design_scores_gemma":[0.0000021762737,0.000030448886,0.9964024,0.000001321671,0.000007723879,0.00014107098,0.000053969346,0.00020548307,0.0028184021,0.000043577977,0.0002919189,0.0000015974249],"about_ca_topic_score_codex":0.0041922987,"about_ca_topic_score_gemma":0.0077211126,"teacher_disagreement_score":0.0041922987,"about_ca_system_score_codex":0.00011968015,"about_ca_system_score_gemma":0.000084944266,"threshold_uncertainty_score":0.008335769},"labels":[],"label_agreement":null},{"id":"W2067813347","doi":"10.1086/379808","title":"On the Purity of the ZZ Ceti Instability Strip: Discovery of More Pulsating DA White Dwarfs on the Basis of Optical Spectroscopy","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Instability strip; White dwarf; Stars; Spectral line; Spectroscopy; Effective temperature; Atmosphere (unit); Stellar classification","score_opus":0.013333206904144208,"score_gpt":0.2350652936861968,"score_spread":0.22173208678205258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067813347","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873894,0.00015393391,0.00047373422,0.00001546516,0.0000011703406,0.0000032846813,0.000048332062,0.000012079294,0.00055299327],"genre_scores_gemma":[0.999138,0.000082052364,0.0005483069,0.000013102462,0.000005661283,0.0000034096793,0.00013148332,0.0000039754077,0.00007395358],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998111,0.000019261468,0.00001920113,0.000058326685,0.00006145585,0.000030661464],"domain_scores_gemma":[0.99904364,0.00024624198,0.00037777863,0.00011755857,0.00010472222,0.00011013368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038248292,0.0002147409,0.00030299276,0.0012968583,0.00048856006,0.0011974627,0.00029998505,0.00023687996,0.000592643],"category_scores_gemma":[0.0014781386,0.0001454326,0.00015465259,0.0010176493,0.00048700222,0.0004046369,0.00078063,0.00025966775,0.00018900333],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023983548,0.000026486283,0.91884756,0.000031515607,0.000031527055,0.00029598648,0.00039700832,0.00026193805,0.06547064,0.00059467147,0.00004733819,0.013755517],"study_design_scores_gemma":[0.000007968206,0.00005917242,0.9888136,0.000004226945,0.000024988316,0.00088728167,0.00015151636,0.0007456506,0.008191206,0.0003592927,0.0007498029,0.000005295677],"about_ca_topic_score_codex":0.00064976234,"about_ca_topic_score_gemma":0.0010306427,"teacher_disagreement_score":0.0012968583,"about_ca_system_score_codex":0.000208726,"about_ca_system_score_gemma":0.00013346072,"threshold_uncertainty_score":0.0020228028},"labels":[],"label_agreement":null},{"id":"W2067819575","doi":"10.1088/0004-637x/733/1/65","title":"CLOUDS AND CHEMISTRY IN THE ATMOSPHERE OF EXTRASOLAR PLANET HR8799b","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":359,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Exoplanet; Physics; Planet; Astrophysics; Surface gravity; Photometry (optics); Atmosphere (unit); Opacity; Metallicity; Spectral line; Astronomy; Stars","score_opus":0.01242574756795202,"score_gpt":0.2030392181563674,"score_spread":0.19061347058841538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067819575","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985599,0.00020637191,0.000083978804,0.00003366305,0.0000035127414,0.0000014061885,0.00022795197,0.000016130003,0.000867079],"genre_scores_gemma":[0.9988977,0.000111427835,0.00015733308,0.000022533257,0.000005024302,0.0000022125796,0.00060002616,0.0000061736,0.00019764274],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999547,0.000006854798,0.0000026585465,0.0000112184935,0.0000125762135,0.000011992103],"domain_scores_gemma":[0.9999311,0.000008112764,0.000027980108,0.0000074290942,0.000008559581,0.00001677199],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009873786,0.0001569234,0.00019781663,0.0004980979,0.00038577884,0.00043249974,0.00017291021,0.00021330325,0.0005526512],"category_scores_gemma":[0.00016109142,0.0001242359,0.0001680293,0.00043893635,0.00015408162,0.0002513298,0.00037912064,0.00021277858,0.00021693132],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003652421,0.00017644327,0.85634786,0.000086692475,0.00018484978,0.0008128292,0.00045538245,0.005487466,0.1196949,0.0012494406,0.00096158707,0.014177271],"study_design_scores_gemma":[0.000014884689,0.00003317869,0.992708,0.0000060303373,0.000015716387,0.00009587964,0.000056421417,0.0042348467,0.0017400008,0.0002143758,0.000876811,0.0000038071403],"about_ca_topic_score_codex":0.0074826027,"about_ca_topic_score_gemma":0.008699603,"teacher_disagreement_score":0.0074826027,"about_ca_system_score_codex":0.00041886693,"about_ca_system_score_gemma":0.00010132183,"threshold_uncertainty_score":0.014878094},"labels":[],"label_agreement":null},{"id":"W2067824076","doi":"10.1088/0004-637x/735/2/109","title":"SECULAR CHAOS AND THE PRODUCTION OF HOT JUPITERS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":438,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Hot Jupiter; Physics; Planet; Astrophysics; Planetary migration; Planetary system; Giant planet; Astronomy; Gas giant; Exoplanet","score_opus":0.00964207549778319,"score_gpt":0.1821409240886758,"score_spread":0.1724988485908926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067824076","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984004,0.00035072904,0.00036121608,0.000048436417,0.000002358659,0.0000028818365,0.000022886967,0.0000073409997,0.0008037396],"genre_scores_gemma":[0.9995142,0.00011530169,0.00016338206,0.0000064631126,0.0000036824863,0.0000020283644,0.000022967848,0.0000015997783,0.00017039657],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999325,0.0000100024845,0.000003997121,0.000015584856,0.000014668177,0.00002318762],"domain_scores_gemma":[0.9992526,0.00010092828,0.00041780283,0.000050364688,0.000036074674,0.00014226683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015723148,0.00012682867,0.00013834414,0.00043924522,0.0003038044,0.00051185983,0.00012087442,0.00017317041,0.0006528937],"category_scores_gemma":[0.00068285555,0.000101970276,0.00009696956,0.00026965933,0.0006190909,0.00030350938,0.000776165,0.00019685419,0.000073606854],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007212858,0.00012381852,0.66077065,0.00021516095,0.00011007503,0.0034985326,0.0042840885,0.0072949557,0.26745015,0.014206062,0.0008850295,0.040440142],"study_design_scores_gemma":[0.000024519131,0.0003266441,0.9478196,0.00002671653,0.000029250894,0.0019941956,0.00074977614,0.008586963,0.023454059,0.013051648,0.0039099194,0.000026768455],"about_ca_topic_score_codex":0.00055414095,"about_ca_topic_score_gemma":0.00052541256,"teacher_disagreement_score":0.0006528937,"about_ca_system_score_codex":0.00028401142,"about_ca_system_score_gemma":0.0001197652,"threshold_uncertainty_score":0.002184093},"labels":[],"label_agreement":null},{"id":"W2067873680","doi":"10.1088/0004-637x/794/1/56","title":"PERPENDICULAR DIFFUSION OF ENERGETIC PARTICLES IN NOISY REDUCED MAGNETOHYDRODYNAMIC TURBULENCE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Magnetohydrodynamic drive; Physics; Perpendicular; Turbulence; Diffusion; Magnetohydrodynamic turbulence; Statistical physics; Magnetic field; Random walk; Classical mechanics; Mechanics; Computational physics; Magnetohydrodynamics; Mathematics; Geometry; Thermodynamics; Quantum mechanics; Statistics","score_opus":0.003277426700433646,"score_gpt":0.19845813812647883,"score_spread":0.19518071142604518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067873680","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.77445066,0.00048823748,0.21523912,0.00083487085,0.00017185474,0.000062098065,0.00020016599,0.0002128808,0.008340198],"genre_scores_gemma":[0.9917006,0.000113918795,0.005791984,0.000049403745,0.000034310116,0.000028686212,0.00006854342,0.000024820165,0.0021877561],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979585,0.00006147908,0.000011052949,0.000036075497,0.00005359355,0.000041877374],"domain_scores_gemma":[0.9996942,0.00008628938,0.00007426538,0.00003252757,0.00005904267,0.000053714175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004523894,0.000527839,0.0006787653,0.0005024962,0.00050686847,0.0012389265,0.0008437069,0.0008757535,0.0005741943],"category_scores_gemma":[0.0013164242,0.00035054135,0.00059199834,0.00026765093,0.0012443993,0.0013520296,0.0008275794,0.00064325845,0.00008784511],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031742896,0.000097608565,0.0030955763,0.000068589405,0.00006479358,0.0005139741,0.00017971633,0.7473496,0.021529505,0.22389002,0.00081301533,0.002080105],"study_design_scores_gemma":[0.000015217558,0.000010072178,0.00030164883,0.000001057098,0.000002705502,0.000016097627,0.0000066317657,0.99289376,0.0002914202,0.006368424,0.00008450472,0.00000835851],"about_ca_topic_score_codex":0.004424644,"about_ca_topic_score_gemma":0.0014629832,"teacher_disagreement_score":0.004424644,"about_ca_system_score_codex":0.0008506293,"about_ca_system_score_gemma":0.0004907058,"threshold_uncertainty_score":0.008797765},"labels":[],"label_agreement":null},{"id":"W2067874668","doi":"10.1088/0004-637x/782/1/8","title":"NEAR-INFRARED (<i>JHK</i>) SPECTROSCOPY OF YOUNG STELLAR AND SUBSTELLAR OBJECTS IN ORION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Stellar classification; Astrophysics; Brown dwarf; Spectral energy distribution; Young stellar object; Stars; Astronomy; Pleiades; Hertzsprung–Russell diagram; Orion Nebula; Extinction (optical mineralogy); Spectrograph; Infrared telescope; Spectral line; Telescope; Star formation; Stellar evolution","score_opus":0.005806952794553969,"score_gpt":0.218206830801386,"score_spread":0.21239987800683202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067874668","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965906,0.00003873155,0.00009248808,0.0000032271535,6.663082e-7,0.0000017574516,0.000031696625,0.0000063885395,0.00016603142],"genre_scores_gemma":[0.9984981,0.000050976352,0.00079213997,0.000009954786,0.0000047683934,0.000006815774,0.00031899713,0.0000069558264,0.00031124495],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998265,0.000013233494,0.000011618597,0.000066388326,0.00004431784,0.000038063987],"domain_scores_gemma":[0.99962795,0.000036428442,0.00014250279,0.00004446821,0.00005140257,0.00009731228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037791862,0.00030590312,0.000292174,0.0011414341,0.00061937154,0.0004457618,0.00055671146,0.00028028607,0.0004510584],"category_scores_gemma":[0.00050459726,0.0002394395,0.0002142243,0.0006409321,0.0002976677,0.00034453196,0.00070501474,0.00021382923,0.00018958215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022079724,0.00010084867,0.8349288,0.000047987087,0.00006257395,0.00038263405,0.0008221619,0.0006539205,0.1518188,0.00013268362,0.00010380515,0.010725037],"study_design_scores_gemma":[0.0000037507295,0.000046047622,0.9959216,0.0000023746375,0.000014946438,0.00013195652,0.00009379794,0.00042693855,0.0030645924,0.000029675764,0.0002603246,0.000004051482],"about_ca_topic_score_codex":0.0032109134,"about_ca_topic_score_gemma":0.0046143834,"teacher_disagreement_score":0.0032109134,"about_ca_system_score_codex":0.00041983253,"about_ca_system_score_gemma":0.0001496769,"threshold_uncertainty_score":0.0063844323},"labels":[],"label_agreement":null},{"id":"W2067881197","doi":"10.1086/421264","title":"The Faintness of the 158 Micron [C <scp>ii</scp> ] Transition in the <i>z</i> =6.42 Quasar SDSS J1148+5251","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Red shift; OVV quasar; Infrared; Transition (genetics); Emission spectrum; Luminosity; Accretion disc","score_opus":0.005057600433496021,"score_gpt":0.19523577030057224,"score_spread":0.19017816986707622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067881197","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99221754,0.00017970247,0.00018429622,0.00034173063,0.00004445544,0.0000042204256,0.000683621,0.00008169693,0.0062626787],"genre_scores_gemma":[0.99758875,0.000044498316,0.000087578315,0.00009648152,0.000037025147,0.000002500417,0.0005923046,0.000017881786,0.0015330092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999124,0.0000055378155,0.000003511165,0.00003270527,0.000018477773,0.000027460006],"domain_scores_gemma":[0.9991334,0.00012572338,0.00029272347,0.000044349294,0.00015692375,0.0002468199],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016994952,0.0001153319,0.00014680708,0.0008872755,0.00042630843,0.0005150219,0.0002282704,0.0005096773,0.008798566],"category_scores_gemma":[0.0009086525,0.00012445099,0.00010877062,0.00036535115,0.0003021268,0.0003317913,0.00030665912,0.0004120902,0.0011131825],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056588254,0.00010194272,0.8132205,0.00012408978,0.00005073767,0.0005587069,0.00044747003,0.0003393547,0.15186103,0.0016839658,0.006344021,0.02470229],"study_design_scores_gemma":[0.000006677903,0.000019456047,0.99754024,0.0000036076017,0.0000056704034,0.00008378543,0.00005618783,0.0001103515,0.0012643569,0.0001317019,0.0007750316,0.0000031349605],"about_ca_topic_score_codex":0.004598829,"about_ca_topic_score_gemma":0.006543321,"teacher_disagreement_score":0.008798566,"about_ca_system_score_codex":0.00020459175,"about_ca_system_score_gemma":0.00011229201,"threshold_uncertainty_score":0.029434144},"labels":[],"label_agreement":null},{"id":"W2067985326","doi":"10.1088/0004-637x/755/2/178","title":"AN OBSERVED LACK OF SUBSTRUCTURE IN STARLESS CORES. II. SUPER-JEANS CORES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Substructure; Thermal; Spectral line; Line (geometry); Core (optical fiber)","score_opus":0.04207959187529078,"score_gpt":0.28305080361358714,"score_spread":0.24097121173829636,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2067985326","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877053,0.000106986794,0.00013780677,0.000011742868,0.0000021671883,0.00000333202,0.0001077747,0.0000097842485,0.0008498823],"genre_scores_gemma":[0.9995616,0.00001652407,0.00010325111,0.000010587957,0.0000028495554,9.174039e-7,0.000145014,0.0000016031041,0.0001575533],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991167,0.000004119051,0.000008105329,0.000031559506,0.000019641113,0.00002484423],"domain_scores_gemma":[0.9990839,0.0000786504,0.0004154041,0.000075799246,0.00011352822,0.00023279666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011690563,0.00015321079,0.00014755032,0.00066885276,0.00025354818,0.00041381287,0.00028169088,0.00020408965,0.0020937885],"category_scores_gemma":[0.00058035494,0.00009583775,0.000086810185,0.00032747627,0.00044319205,0.00025210332,0.00039621093,0.0001552705,0.0003548754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023493328,0.000051113817,0.9264297,0.00003504044,0.000026632255,0.0006479284,0.00023284616,0.00014464684,0.06562276,0.00031145886,0.0001727823,0.006090193],"study_design_scores_gemma":[0.000011498298,0.000081073835,0.99263495,0.0000045455463,0.000008399299,0.0013254671,0.00013236764,0.00032184867,0.004670151,0.00025383738,0.0005524808,0.000003269317],"about_ca_topic_score_codex":0.0017265682,"about_ca_topic_score_gemma":0.0034171313,"teacher_disagreement_score":0.0020937885,"about_ca_system_score_codex":0.0001691304,"about_ca_system_score_gemma":0.00011526758,"threshold_uncertainty_score":0.00700444},"labels":[],"label_agreement":null},{"id":"W2068008066","doi":"10.1088/0004-637x/751/2/158","title":"MIGRATION THEN ASSEMBLY: FORMATION OF NEPTUNE-MASS PLANETS INSIDE 1 AU","year":2012,"lang":"fr","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":307,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Neptune; Planet; Physics; Astrophysics; Mass distribution; Accretion (finance); Nebula; Astronomy; Stars","score_opus":0.015136669572109202,"score_gpt":0.2233823633887864,"score_spread":0.20824569381667718,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068008066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99706346,0.00007132761,0.0012296005,0.000050546343,0.0000031552202,0.00000235655,0.0000691232,0.000030465486,0.0014798112],"genre_scores_gemma":[0.9992737,0.00002506866,0.00038069676,0.000005624128,0.000001372461,0.0000020079758,0.00007508434,0.0000044033072,0.00023209091],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999443,0.0000069135117,0.000001798012,0.000023768225,0.0000054005195,0.000017777777],"domain_scores_gemma":[0.9998004,0.00004509974,0.00006906129,0.0000278778,0.000012481691,0.00004516167],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001354881,0.00023091368,0.00016158848,0.0002564491,0.00035213516,0.00046166964,0.00045240988,0.00037154392,0.0012813788],"category_scores_gemma":[0.0006250732,0.00013721509,0.00026336382,0.00022480442,0.00026244193,0.00037972507,0.00033536693,0.00024491837,0.00027906243],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070965383,0.00009302607,0.79395616,0.000096687254,0.000093363175,0.001599312,0.0011527049,0.11407445,0.050490085,0.013294847,0.0018564962,0.022583233],"study_design_scores_gemma":[0.000061147286,0.00023546282,0.42505032,0.000017414148,0.00005742295,0.0017552873,0.0008488096,0.54875946,0.012747404,0.0057737934,0.004655666,0.000037787107],"about_ca_topic_score_codex":0.0069097774,"about_ca_topic_score_gemma":0.00466689,"teacher_disagreement_score":0.0069097774,"about_ca_system_score_codex":0.0004471208,"about_ca_system_score_gemma":0.00012523858,"threshold_uncertainty_score":0.013739109},"labels":[],"label_agreement":null},{"id":"W2068041806","doi":"10.1088/0004-637x/751/2/102","title":"NUCLEOSYNTHESIS AND THE INHOMOGENEOUS CHEMICAL EVOLUTION OF THE CARINA DWARF GALAXY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":167,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Science and Technology Facilities Council; University of Victoria; National Science Foundation","keywords":"Astrophysics; Physics; Stars; Nucleosynthesis; Galaxy; Dwarf galaxy; Halo; Population; Metallicity; Star formation; Dwarf spheroidal galaxy; Spectral line; Galactic halo; Astronomy","score_opus":0.0065338949078231545,"score_gpt":0.19361007275987607,"score_spread":0.1870761778520529,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068041806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992508,0.00027106397,0.000093050636,0.0000047816325,4.8371226e-7,9.630883e-7,0.000028551247,0.0000037048248,0.00034648835],"genre_scores_gemma":[0.99958557,0.000084723826,0.00013200619,0.0000032515957,0.0000010817199,0.0000010458845,0.00006534549,0.000001850182,0.00012513217],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999403,0.000009432001,0.0000029698165,0.000025227651,0.000009852738,0.000012175386],"domain_scores_gemma":[0.99979967,0.00003859109,0.00007577511,0.000019726498,0.000026398733,0.000039899118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013725107,0.00023234742,0.00014315704,0.00061775005,0.0002609327,0.00046078398,0.00023920994,0.00015413012,0.00039245535],"category_scores_gemma":[0.0003724191,0.00014560702,0.00012511207,0.00029277964,0.00033360493,0.0001921465,0.00029675415,0.00009500798,0.0001253086],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024206865,0.000017868448,0.88016963,0.000040557486,0.000065944536,0.00031079145,0.00058763276,0.001932615,0.10515545,0.0006716455,0.000042186468,0.010763574],"study_design_scores_gemma":[0.0000035955838,0.000050865714,0.9919613,0.0000032625805,0.000020021918,0.0002106374,0.00017488403,0.0017281913,0.004727661,0.00015124244,0.0009632317,0.000005022071],"about_ca_topic_score_codex":0.013656682,"about_ca_topic_score_gemma":0.015283094,"teacher_disagreement_score":0.013656682,"about_ca_system_score_codex":0.00068491115,"about_ca_system_score_gemma":0.00017407098,"threshold_uncertainty_score":0.027154386},"labels":[],"label_agreement":null},{"id":"W2068048529","doi":"10.1086/381674","title":"1420 MHz Continuum Absorption toward Extragalactic Sources in the Galactic Plane","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary","funders":"","keywords":"Astrophysics; Galactic plane; Physics; Absorption (acoustics); RADIUS; Spectral line; Absorption spectroscopy; Emission spectrum; Galaxy; Astronomy; Optics","score_opus":0.013743645131374414,"score_gpt":0.2384835867549957,"score_spread":0.2247399416236213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068048529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99821055,0.00015692989,0.00011055452,0.000017119826,0.0000011018822,0.0000032503078,0.0004952476,0.0000098743785,0.0009953888],"genre_scores_gemma":[0.9972372,0.00024157096,0.00028303737,0.000014490815,0.000008303681,0.0000030640317,0.0014429752,0.000005141079,0.00076418574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997652,0.0000143895395,0.000004772264,0.00004570148,0.00008463189,0.00008525565],"domain_scores_gemma":[0.9994375,0.000049648206,0.0001338094,0.00003224865,0.00020218205,0.00014464563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019004203,0.00025350443,0.00020307156,0.0018479924,0.00073773996,0.00053113844,0.00032932314,0.00017583693,0.0012803607],"category_scores_gemma":[0.0005677682,0.0001566637,0.00017198201,0.002292329,0.0003027372,0.0002055289,0.00040460314,0.00014161498,0.00025911772],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009151933,0.00003132072,0.97902334,0.00002513179,0.00004643391,0.00017323895,0.0005160858,0.00031293413,0.0072248084,0.00013379873,0.00028984103,0.0121315],"study_design_scores_gemma":[0.0000012144615,0.000006049096,0.9992016,0.0000013506333,0.0000062812405,0.00005469092,0.000050830888,0.00007834695,0.0002224392,0.000012017152,0.00036355166,0.0000016227008],"about_ca_topic_score_codex":0.41740182,"about_ca_topic_score_gemma":0.5653647,"teacher_disagreement_score":0.41740182,"about_ca_system_score_codex":0.0013056446,"about_ca_system_score_gemma":0.0006388126,"threshold_uncertainty_score":0.82994455},"labels":[],"label_agreement":null},{"id":"W2068050609","doi":"10.1088/0004-637x/740/2/88","title":"MODES OF STAR FORMATION IN FINITE MOLECULAR CLOUDS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Molecular cloud; Star formation; Context (archaeology); Gravitational collapse; Enhanced Data Rates for GSM Evolution; Star (game theory)","score_opus":0.018137945055018218,"score_gpt":0.2310087801590793,"score_spread":0.21287083510406107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068050609","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9643934,0.00023912684,0.027520042,0.00018174831,0.000015579113,0.00003775473,0.000057304955,0.00005472271,0.0075002587],"genre_scores_gemma":[0.9979705,0.000086864486,0.0015066531,0.000015032308,0.0000058618234,0.000016295333,0.000020270743,0.0000075239245,0.000370934],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998149,0.0000393322,0.0000072016046,0.000014538071,0.00005003063,0.00007396354],"domain_scores_gemma":[0.99943286,0.00018985065,0.00014999928,0.00004268522,0.00006190226,0.00012266109],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004608035,0.00033623562,0.00036521084,0.00064764725,0.00070253754,0.0010785497,0.00072317675,0.000492689,0.00097153906],"category_scores_gemma":[0.002212242,0.0002292539,0.0005189476,0.0003152923,0.0018614818,0.0010646502,0.0007213304,0.00039367483,0.000084532156],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007867665,0.000045273147,0.004717415,0.000039339167,0.000024679244,0.0002837506,0.00019880179,0.8976267,0.0034941533,0.09200283,0.00017009348,0.0013182262],"study_design_scores_gemma":[0.000033542776,0.000027323345,0.0012768507,0.000009603113,0.000006967111,0.00005711633,0.00007818008,0.97672105,0.0004337652,0.021084828,0.00025776666,0.000012972791],"about_ca_topic_score_codex":0.009460371,"about_ca_topic_score_gemma":0.0035930888,"teacher_disagreement_score":0.009460371,"about_ca_system_score_codex":0.0016928441,"about_ca_system_score_gemma":0.0008868762,"threshold_uncertainty_score":0.01881057},"labels":[],"label_agreement":null},{"id":"W2068129589","doi":"10.1086/513309","title":"The Distance to the Isolated Neutron Star RX J0720.4−3125","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Parallax; Proper motion; Measure (data warehouse); Neutron star; Advanced Camera for Surveys; Telescope; Position (finance); Star (game theory)","score_opus":0.008225676378411232,"score_gpt":0.3073030906455801,"score_spread":0.2990774142671689,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068129589","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99420035,0.00042686434,0.00068767,0.000038779428,0.000016853252,0.000009407454,0.0012189202,0.000039437706,0.0033617374],"genre_scores_gemma":[0.9916544,0.00016982757,0.0016246199,0.000041854666,0.000025622678,0.0000111987165,0.0050625876,0.000026018532,0.001383952],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999724,0.000024887986,0.000022089504,0.000115502,0.00007299028,0.000040674287],"domain_scores_gemma":[0.9994373,0.000048869846,0.0001952817,0.000056656503,0.00010595555,0.00015600011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041281522,0.00027919735,0.00029595825,0.0009659362,0.0005009758,0.00045362092,0.00040901772,0.000290975,0.0018552806],"category_scores_gemma":[0.0008615711,0.00012573182,0.00020478066,0.00083612336,0.00021642186,0.00024212617,0.0006564373,0.00039550336,0.00086980785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028796805,0.00010043316,0.875932,0.0001741917,0.0001601181,0.00035954855,0.0005071874,0.0016995003,0.09346245,0.0014856167,0.001366921,0.024464041],"study_design_scores_gemma":[0.000008339168,0.00010983861,0.99102134,0.000014479525,0.000028006534,0.0003451711,0.00007419829,0.0007004012,0.0031282608,0.00014964456,0.0044084257,0.000011940079],"about_ca_topic_score_codex":0.0049674134,"about_ca_topic_score_gemma":0.0108287055,"teacher_disagreement_score":0.0049674134,"about_ca_system_score_codex":0.00050944753,"about_ca_system_score_gemma":0.00033810447,"threshold_uncertainty_score":0.009877026},"labels":[],"label_agreement":null},{"id":"W2068149521","doi":"10.1086/587433","title":"The Globular Cluster Systems around NGC 3311 and NGC 3309","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Globular cluster; Physics; Metallicity; Astronomy; Galaxy; Photometry (optics); Elliptical galaxy","score_opus":0.007816204307958891,"score_gpt":0.19796909461063475,"score_spread":0.19015289030267585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068149521","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977552,0.000073951946,0.000073683026,0.000011937538,0.0000015236045,0.000007111289,0.00045322187,0.0000150112455,0.001608286],"genre_scores_gemma":[0.9982273,0.000043358752,0.00024426487,0.000008493876,0.0000025178488,0.0000053817585,0.0011432383,0.0000035602845,0.00032185324],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998419,0.000012678799,0.0000053062085,0.000046102305,0.000039985218,0.00005397693],"domain_scores_gemma":[0.9997167,0.000025348101,0.000085827276,0.000027333124,0.000034382763,0.000110390174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013325257,0.0002352742,0.00014144115,0.0011403201,0.00047025725,0.00039878616,0.00020095952,0.00018016195,0.0013946181],"category_scores_gemma":[0.00032239346,0.00015305194,0.00009334182,0.0011390921,0.00036425292,0.00023391224,0.00091317605,0.00021274247,0.00029271125],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003495505,0.00006451843,0.9451786,0.000091443115,0.000046214493,0.00047511305,0.002203199,0.0008651734,0.030507172,0.00090521184,0.0019361583,0.017377524],"study_design_scores_gemma":[0.0000025917066,0.000020388965,0.99816257,0.0000037867599,0.000003890701,0.000117240925,0.00016158368,0.0001037696,0.00020256719,0.000036112695,0.0011824014,0.0000030460278],"about_ca_topic_score_codex":0.02434987,"about_ca_topic_score_gemma":0.04097186,"teacher_disagreement_score":0.02434987,"about_ca_system_score_codex":0.0006527011,"about_ca_system_score_gemma":0.00027513402,"threshold_uncertainty_score":0.048416257},"labels":[],"label_agreement":null},{"id":"W2068167251","doi":"10.1086/321395","title":"Weak‐Lensing Measurements of 42 SDSS/RASS Galaxy Clusters","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Sky; ROSAT; Weak gravitational lensing; Photometry (optics); Galaxy; Redshift; Galaxy cluster; Cluster (spacecraft); Stars","score_opus":0.018617277454165575,"score_gpt":0.22875021920314362,"score_spread":0.21013294174897804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068167251","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991934,0.00003201377,0.00010602035,0.000007591481,7.0678e-7,0.0000031585307,0.00027909342,0.000013918147,0.0003640854],"genre_scores_gemma":[0.9973023,0.00004063373,0.0005970918,0.000009062134,0.000007798916,0.0000061180135,0.0017046133,0.00001190635,0.0003204441],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994831,0.00005803931,0.00003303245,0.00014674757,0.00015752562,0.00012155629],"domain_scores_gemma":[0.9983903,0.00012880797,0.00036075024,0.00028067944,0.00037320796,0.0004662422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050767674,0.00032693907,0.00040222576,0.0018959489,0.0010224165,0.00060901494,0.0003789461,0.00020130012,0.0008836531],"category_scores_gemma":[0.0016953538,0.00034784703,0.00021065478,0.001358251,0.00030657407,0.0003676111,0.00085498043,0.00027169316,0.00044835018],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001687973,0.000052505937,0.9569347,0.000021908343,0.00007349291,0.0001739812,0.0011552734,0.0008646964,0.029232182,0.00033045444,0.0006055512,0.010386589],"study_design_scores_gemma":[0.000004841002,0.000040757415,0.9955043,0.0000013444887,0.000012248945,0.00012505068,0.00013740512,0.00065742136,0.0026238896,0.00006508509,0.0008200806,0.0000076094025],"about_ca_topic_score_codex":0.014858161,"about_ca_topic_score_gemma":0.020451797,"teacher_disagreement_score":0.014858161,"about_ca_system_score_codex":0.00065302866,"about_ca_system_score_gemma":0.00023504798,"threshold_uncertainty_score":0.02954334},"labels":[],"label_agreement":null},{"id":"W2068208366","doi":"10.1086/505461","title":"Discovery of 14 Radio Pulsars in a Survey of the Magellanic Clouds","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Large Magellanic Cloud; Galaxy; Luminosity; Astronomy; Radio telescope; Small Magellanic Cloud; Luminosity function","score_opus":0.011164789030343864,"score_gpt":0.2860634047112969,"score_spread":0.27489861568095303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068208366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999526,0.00011540118,0.00009562652,0.00002252044,0.000002521661,0.0000045391976,0.000060909544,0.0000040824057,0.00016835766],"genre_scores_gemma":[0.99823356,0.00033240317,0.00048798727,0.00005381307,0.000019857172,0.0000110261035,0.00045945693,0.0000031809736,0.0003986619],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954504,0.00005134843,0.00003620809,0.00009188641,0.00014259294,0.00013287421],"domain_scores_gemma":[0.9986218,0.0002005807,0.0004895688,0.00012011834,0.00020236142,0.00036558765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004709016,0.00021658454,0.00035434277,0.001885568,0.0008626538,0.0008406378,0.00038101358,0.00031333612,0.0004997362],"category_scores_gemma":[0.0015685682,0.0003084983,0.0001428843,0.0015842016,0.0005522502,0.0004348951,0.0009029903,0.0002877432,0.00021885554],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004526022,0.000032098524,0.9873043,0.000012084554,0.000018853705,0.00029131386,0.00039375245,0.000039967457,0.005290127,0.000057657297,0.00010254948,0.0064121187],"study_design_scores_gemma":[0.000006739706,0.00006704943,0.99732506,0.0000046910673,0.000016822092,0.00058149896,0.00021328047,0.00008462556,0.00043833337,0.000037948234,0.0012194521,0.000004499221],"about_ca_topic_score_codex":0.004633262,"about_ca_topic_score_gemma":0.008399686,"teacher_disagreement_score":0.004633262,"about_ca_system_score_codex":0.00036311516,"about_ca_system_score_gemma":0.00043034722,"threshold_uncertainty_score":0.0092125535},"labels":[],"label_agreement":null},{"id":"W2068289629","doi":"10.1088/0004-637x/780/2/144","title":"PROPERTIES OF MAGNETIC HELICITY FLUX IN TURBULENT DYNAMOS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Eusko Jaurlaritza","keywords":"Physics; Dynamo; Helicity; Turbulence; Magnetic helicity; Solar dynamo; Magnetic field; Dynamo theory; Magnetohydrodynamic turbulence; Advection; Magnetic flux; Magnetohydrodynamics; Flux (metallurgy); Classical mechanics; Mechanics; Quantum mechanics","score_opus":0.007040307955312994,"score_gpt":0.193905139124079,"score_spread":0.186864831168766,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068289629","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941706,0.000096769014,0.0029594311,0.00020100997,0.000024319828,0.000018544937,0.000117094765,0.000093339,0.0023188887],"genre_scores_gemma":[0.99914646,0.00002982315,0.0005275251,0.000014560268,0.000005488433,0.000010749981,0.00008551091,0.00002516542,0.00015468971],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998938,0.00003109222,0.000007729995,0.00001557265,0.000018507233,0.000033373122],"domain_scores_gemma":[0.99913305,0.00035945242,0.00016800954,0.000056273842,0.00011395252,0.00016914876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049779605,0.00046537718,0.0004595665,0.0005996933,0.00077567477,0.00092131423,0.00040175035,0.00058460253,0.00082282175],"category_scores_gemma":[0.0025621294,0.00033284884,0.0004306353,0.0003588964,0.0011433548,0.00069080474,0.00047350416,0.00059781864,0.00006617382],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004737593,0.00018871235,0.02050637,0.00006801865,0.00010636371,0.0005005516,0.00023794333,0.9494604,0.017520202,0.008370319,0.0005019015,0.0020654292],"study_design_scores_gemma":[0.000055122746,0.000050697403,0.0031763453,0.000008987495,0.000011471503,0.00002511638,0.000044234326,0.99365085,0.0016511147,0.0011771284,0.00013555029,0.000013431744],"about_ca_topic_score_codex":0.0064798067,"about_ca_topic_score_gemma":0.0025707837,"teacher_disagreement_score":0.0064798067,"about_ca_system_score_codex":0.0007959578,"about_ca_system_score_gemma":0.00068388745,"threshold_uncertainty_score":0.01288414},"labels":[],"label_agreement":null},{"id":"W2068303945","doi":"10.1086/525522","title":"Models of Type I X-Ray Bursts from GS 1826-24: A Probe of rp-Process Hydrogen Burning","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Thermonuclear fusion; Nucleosynthesis; Accretion (finance); Metallicity; Hydrogen; Gamma-ray burst; Stellar evolution; Neutron star; Stellar mass; Thermal","score_opus":0.0198366266132967,"score_gpt":0.25102634015514264,"score_spread":0.23118971354184592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068303945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99574137,0.00006672021,0.0020110793,0.00005760127,0.0000040914715,0.000011857507,0.0003307566,0.00008428467,0.0016923362],"genre_scores_gemma":[0.9977508,0.00006825697,0.0010129804,0.0000068170675,0.0000047091107,0.000016524302,0.00042150693,0.000032830296,0.00068555924],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995255,0.000015156934,0.0000033271276,0.000011786032,0.000006592621,0.000010625202],"domain_scores_gemma":[0.9997665,0.00009736903,0.000046956386,0.000026913427,0.00002093357,0.00004120321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019947163,0.00051928504,0.0002863191,0.00031407544,0.0003172903,0.0006413118,0.00084888,0.00046589048,0.0015366173],"category_scores_gemma":[0.00062849163,0.00024012101,0.0005497217,0.0003052718,0.00027579218,0.00038434338,0.0003450441,0.00038975893,0.00023476484],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002831581,0.00008652602,0.040172916,0.0000486219,0.000069001595,0.00020893071,0.00010134234,0.94684964,0.0063675866,0.003091,0.00038743322,0.002333829],"study_design_scores_gemma":[0.000058625967,0.00008630214,0.015856367,0.000004378602,0.000024150184,0.000082714505,0.000047594527,0.98023605,0.0015758047,0.0016267737,0.00038677108,0.000014426222],"about_ca_topic_score_codex":0.009099068,"about_ca_topic_score_gemma":0.0049326695,"teacher_disagreement_score":0.009099068,"about_ca_system_score_codex":0.000964035,"about_ca_system_score_gemma":0.00019808559,"threshold_uncertainty_score":0.018092215},"labels":[],"label_agreement":null},{"id":"W2068340857","doi":"10.1088/0004-637x/753/1/46","title":"LUMINOUS INFRARED GALAXIES WITH THE SUBMILLIMETER ARRAY. III. THE DENSE KILOPARSEC MOLECULAR CONCENTRATIONS OF Arp 299","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Star formation; Radiative transfer; Infrared; Spiral galaxy; James Clerk Maxwell Telescope; Stars; Submillimeter Array; Luminous infrared galaxy","score_opus":0.006894629907293147,"score_gpt":0.19817606824806427,"score_spread":0.19128143834077113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068340857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9130233,0.0015935559,0.018657504,0.0003899957,0.00005545169,0.000118872114,0.012117898,0.0018442747,0.05219919],"genre_scores_gemma":[0.9659435,0.00028282637,0.021617657,0.00020269731,0.0000647171,0.000084608655,0.007936474,0.000089005196,0.003778481],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979943,0.000019665671,0.000006699719,0.00008842023,0.000053698215,0.00003211544],"domain_scores_gemma":[0.9996848,0.00003712152,0.00011776501,0.000077039964,0.000028348444,0.000054939337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000323824,0.0003081958,0.00028057882,0.00074691896,0.00035190326,0.00056904514,0.00057098526,0.0002850338,0.0051582553],"category_scores_gemma":[0.00043151487,0.00026857218,0.0003199656,0.0006812143,0.00016159355,0.00045015165,0.00064262765,0.00052472035,0.0019260609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000718615,0.00031031852,0.67874604,0.00018242317,0.0002301943,0.00059748587,0.0005847861,0.008181967,0.18850255,0.007395863,0.009055035,0.10549479],"study_design_scores_gemma":[0.00006412313,0.0001255288,0.9568253,0.000029391435,0.000057452748,0.00050128554,0.00009870192,0.009587528,0.012729886,0.0018378692,0.018113669,0.000029309898],"about_ca_topic_score_codex":0.003424201,"about_ca_topic_score_gemma":0.0070079686,"teacher_disagreement_score":0.0051582553,"about_ca_system_score_codex":0.0002759655,"about_ca_system_score_gemma":0.00010394051,"threshold_uncertainty_score":0.017256021},"labels":[],"label_agreement":null},{"id":"W2068340869","doi":"10.1086/373919","title":"A New Approach to Galaxy Morphology. I. Analysis of the Sloan Digital Sky Survey Early Data Release","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":436,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Galaxy; Gini coefficient; Sky; Statistic; Astrophysics; Surface brightness; Physics; Fundamental plane (elliptical galaxies); Measure (data warehouse); Sample (material); Galaxy formation and evolution; Statistics; Mathematics; Lenticular galaxy; Computer science; Inequality; Mathematical analysis; Economic inequality","score_opus":0.020748497048723197,"score_gpt":0.23168524397377405,"score_spread":0.21093674692505085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068340869","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.05503731,0.003775591,0.9163351,0.0014134224,0.00022487353,0.00012034374,0.0048212637,0.0015210591,0.016751137],"genre_scores_gemma":[0.5944998,0.0026931486,0.3873285,0.0006272863,0.0006946221,0.0004010132,0.0059069465,0.0006230544,0.0072255908],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9991254,0.00023437486,0.00006125706,0.00023940812,0.00028590072,0.000053733966],"domain_scores_gemma":[0.99801326,0.00049893773,0.00047472713,0.000567173,0.0003339727,0.00011193387],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009304964,0.00058950484,0.00071414915,0.0059331893,0.0006848632,0.0029933979,0.00079478795,0.0005608575,0.0016977659],"category_scores_gemma":[0.0056646173,0.00033839644,0.0011164848,0.00505244,0.0015356103,0.0019647896,0.0016645485,0.0010876672,0.0011379719],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014501261,0.00006962743,0.109501295,0.00030676575,0.00037854823,0.00044935432,0.001079605,0.03700888,0.011410503,0.42464045,0.018157056,0.396853],"study_design_scores_gemma":[0.00003586533,0.00011623892,0.18941306,0.00013861018,0.00009619522,0.0013194345,0.0005876203,0.20464638,0.005165465,0.4520368,0.14633037,0.00011397871],"about_ca_topic_score_codex":0.00700047,"about_ca_topic_score_gemma":0.0035152847,"teacher_disagreement_score":0.00700047,"about_ca_system_score_codex":0.0013100723,"about_ca_system_score_gemma":0.00047114183,"threshold_uncertainty_score":0.013919473},"labels":[],"label_agreement":null},{"id":"W2068422897","doi":"10.1088/0004-637x/738/1/39","title":"ORBITING CIRCUMGALACTIC GAS AS A SIGNATURE OF COSMOLOGICAL ACCRETION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":176,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Accretion (finance); Halo; Angular momentum; Redshift; Galactic halo; Specific relative angular momentum; Intergalactic travel; Active galactic nucleus","score_opus":0.014345104039961929,"score_gpt":0.21842288456459572,"score_spread":0.2040777805246338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068422897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963026,0.0000640768,0.0012735655,0.00013776154,0.0000128202,0.000011413533,0.00017472367,0.00009179295,0.0019312823],"genre_scores_gemma":[0.99758923,0.000041787654,0.0017092953,0.000046638444,0.000009502639,0.000008917662,0.0002668765,0.000028642798,0.00029919323],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99990594,0.000030523744,0.0000036008776,0.000013993112,0.000017002409,0.000028891223],"domain_scores_gemma":[0.99932945,0.00021111943,0.0001498325,0.000055171047,0.000054288354,0.00020014518],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050226226,0.00046953582,0.0003924035,0.0007069902,0.00055604754,0.00085688074,0.00089245784,0.00073214044,0.0013634],"category_scores_gemma":[0.0017858273,0.00033164647,0.000528462,0.00058645534,0.00070242374,0.00053474534,0.0007741163,0.00074766984,0.00013644647],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003227634,0.00026169705,0.0728041,0.000041303945,0.00025027836,0.00047308372,0.00023651039,0.90934366,0.004545248,0.008138361,0.0009211411,0.002661859],"study_design_scores_gemma":[0.00006145501,0.0000411932,0.009374667,0.000004474617,0.000019988523,0.000019107774,0.00005263011,0.98882896,0.0002716362,0.0010485165,0.00026655532,0.000010752215],"about_ca_topic_score_codex":0.031939898,"about_ca_topic_score_gemma":0.020248529,"teacher_disagreement_score":0.031939898,"about_ca_system_score_codex":0.0011309707,"about_ca_system_score_gemma":0.0008062464,"threshold_uncertainty_score":0.063507974},"labels":[],"label_agreement":null},{"id":"W2068441296","doi":"10.1088/0004-637x/713/2/1376","title":"DAMPING OF MAGNETOHYDRODYNAMIC TURBULENCE IN PARTIALLY IONIZED GAS AND THE OBSERVED DIFFERENCE OF VELOCITIES OF NEUTRALS AND IONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Turbulence; Physics; Supersonic speed; Magnetohydrodynamic turbulence; Mach number; Computational physics; Magnetohydrodynamics; K-epsilon turbulence model; Mechanics; Wave turbulence; Classical mechanics; Astrophysics; Plasma; Quantum mechanics","score_opus":0.011668471250969452,"score_gpt":0.22256868269503496,"score_spread":0.2109002114440655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068441296","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9886911,0.00025295452,0.009032265,0.00020347109,0.000012363026,0.00000788892,0.00006533551,0.0001222048,0.0016125134],"genre_scores_gemma":[0.9989072,0.0000498502,0.00094217854,0.000008071098,0.0000028278307,0.0000028018162,0.000019004225,0.000008851323,0.000059180005],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999461,0.000013289616,0.0000037698499,0.000009796419,0.00001427603,0.000012656646],"domain_scores_gemma":[0.99972063,0.0001233652,0.00009221281,0.000020591478,0.000014537962,0.000028588654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019145341,0.0002794269,0.0001457729,0.0003055292,0.00023253556,0.0004916359,0.0003330936,0.00028153785,0.00039516867],"category_scores_gemma":[0.0011570409,0.00016739365,0.00026998628,0.00027555722,0.00064860965,0.00050599186,0.00036515322,0.00033087115,0.000042726686],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063910487,0.00013575965,0.11707973,0.00016996099,0.00009675998,0.00064860086,0.0006128482,0.7342526,0.10248934,0.031408083,0.0004720477,0.011995148],"study_design_scores_gemma":[0.00003312649,0.000060587827,0.042499665,0.000014622735,0.0000098120445,0.00007438825,0.000058873673,0.9467852,0.0058802306,0.0042822897,0.00027953665,0.000021755524],"about_ca_topic_score_codex":0.002858976,"about_ca_topic_score_gemma":0.0012072572,"teacher_disagreement_score":0.002858976,"about_ca_system_score_codex":0.00041518692,"about_ca_system_score_gemma":0.00019581859,"threshold_uncertainty_score":0.0056847334},"labels":[],"label_agreement":null},{"id":"W2068523501","doi":"10.1088/0004-637x/796/2/107","title":"RADIATION FEEDBACK IN ULIRGs: ARE PHOTONS MOVERS AND SHAKERS?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Radiation; Photon; Acceleration; Momentum (technical analysis); Diffusion; Radiation pressure; Turbulence; Field (mathematics); Gravitational field","score_opus":0.004686147871575189,"score_gpt":0.19336267764449722,"score_spread":0.18867652977292204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068523501","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975284,0.00006367805,0.0010999857,0.00010596216,0.000007202533,0.0000108432305,0.00006072917,0.000062802166,0.001060323],"genre_scores_gemma":[0.9990564,0.000026098973,0.00058789685,0.000044657554,0.000004814362,0.0000058375913,0.000061700644,0.000018028593,0.00019456125],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998858,0.000022641841,0.000004422456,0.000022488362,0.000015914535,0.000048695874],"domain_scores_gemma":[0.99938834,0.00019581817,0.000131797,0.000041389743,0.000048317943,0.00019431987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042232487,0.0005074532,0.0004856604,0.00038542447,0.0007241843,0.0010320625,0.0008916928,0.00080765213,0.00092707225],"category_scores_gemma":[0.0017908189,0.0002684547,0.0005760761,0.00034132955,0.0008766789,0.0007637281,0.00068077754,0.00072445837,0.000085915155],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051075843,0.0004161664,0.21683149,0.00011447982,0.00020613859,0.0017386691,0.0011244094,0.7325355,0.026690543,0.011114846,0.0010463969,0.0076706037],"study_design_scores_gemma":[0.00014468339,0.00014728453,0.03733367,0.000022261593,0.00004229579,0.00009733326,0.00042913103,0.9557338,0.002703364,0.0027415059,0.0005704467,0.000034261713],"about_ca_topic_score_codex":0.01811135,"about_ca_topic_score_gemma":0.008744541,"teacher_disagreement_score":0.01811135,"about_ca_system_score_codex":0.001022281,"about_ca_system_score_gemma":0.0005129872,"threshold_uncertainty_score":0.036011875},"labels":[],"label_agreement":null},{"id":"W2068549128","doi":"10.1086/587926","title":"Testing Modified Gravity with Globular Cluster Velocity Dispersions","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Globular cluster; Modified Newtonian dynamics; Physics; Velocity dispersion; Astrophysics; Galaxy rotation curve; Galaxy; Milky Way; Gravitation; Newtonian fluid; Newtonian dynamics; Astronomy; Classical mechanics; Halo","score_opus":0.014274856105354512,"score_gpt":0.2084872528756616,"score_spread":0.1942123967703071,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068549128","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99027014,0.00010668658,0.004765305,0.00022056191,0.000024978108,0.000022715925,0.00028309235,0.00009666423,0.00420991],"genre_scores_gemma":[0.9981458,0.000024818692,0.0014278638,0.00003488733,0.00001900001,0.000011662289,0.00016550222,0.000019777546,0.00015068302],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9951332,0.0022000151,0.0002309882,0.0010811894,0.0010274443,0.00032715962],"domain_scores_gemma":[0.9129987,0.06063186,0.012604733,0.007936181,0.0033534209,0.0024751276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.006316205,0.0014274265,0.00054046937,0.0019371299,0.0009166534,0.0022619092,0.002031888,0.0012729785,0.0029730517],"category_scores_gemma":[0.07720436,0.00033094434,0.0009895778,0.0019559294,0.0036098557,0.0037195503,0.002929278,0.001011591,0.0006096384],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008146396,0.0002572897,0.9352498,0.00005714515,0.00051080744,0.00023975428,0.0009422744,0.024623005,0.0011439248,0.019579995,0.00087496353,0.015706362],"study_design_scores_gemma":[0.000334161,0.0016971822,0.5846756,0.00007659687,0.00041737978,0.00045732758,0.0014023718,0.3043315,0.0041137356,0.09781274,0.0045309197,0.00015052076],"about_ca_topic_score_codex":0.0088893045,"about_ca_topic_score_gemma":0.0028678882,"teacher_disagreement_score":0.0088893045,"about_ca_system_score_codex":0.0017049423,"about_ca_system_score_gemma":0.000708015,"threshold_uncertainty_score":0.033403635},"labels":[],"label_agreement":null},{"id":"W2068649880","doi":"10.1086/312885","title":"Magnetic Fields and the Triaxiality of Molecular Cloud Cores","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Magnetic field; Offset (computer science); Flattening; Molecular cloud; Physics; Polarization (electrochemistry); Cloud computing; Computational physics; Statistical physics; Astrophysics; Astronomy; Computer science; Quantum mechanics","score_opus":0.0063392628696070895,"score_gpt":0.22264160034880146,"score_spread":0.21630233747919436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068649880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998601,0.000047298767,0.00059615396,0.000019805368,8.568286e-7,0.000003041826,0.00004433014,0.000008840175,0.00067860313],"genre_scores_gemma":[0.99975675,0.000020783002,0.00012986429,0.000002148992,0.0000014730996,0.0000011870104,0.00005834738,0.0000027441556,0.000026829672],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980754,0.000028657036,0.0000092526825,0.0000424974,0.000040052808,0.00007195335],"domain_scores_gemma":[0.99771214,0.00057725795,0.0010912145,0.00018894537,0.00018250517,0.00024801842],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032515798,0.00014899255,0.00016932887,0.0006695409,0.0004751144,0.0008401933,0.00032453577,0.00022931093,0.0011936835],"category_scores_gemma":[0.003123297,0.00018084505,0.00017397758,0.00060392893,0.0007265959,0.0006058022,0.00059570814,0.0003034851,0.00014440533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073220686,0.00007609439,0.91647243,0.000035962206,0.00008331168,0.00029192862,0.00033587468,0.046098933,0.019828554,0.0059067034,0.00033977957,0.009798212],"study_design_scores_gemma":[0.00010839995,0.0002720978,0.8491647,0.000025233408,0.00006367146,0.00068865524,0.0004979604,0.13317175,0.010103437,0.004682342,0.0011770457,0.00004463748],"about_ca_topic_score_codex":0.0032679632,"about_ca_topic_score_gemma":0.003031731,"teacher_disagreement_score":0.0032679632,"about_ca_system_score_codex":0.0004710089,"about_ca_system_score_gemma":0.00022497617,"threshold_uncertainty_score":0.0064979196},"labels":[],"label_agreement":null},{"id":"W2068718676","doi":"10.1088/0004-637x/729/2/88","title":"PUSHING THE BOUNDARIES OF CONVENTIONAL CORE-COLLAPSE SUPERNOVAE: THE EXTREMELY ENERGETIC SUPERNOVA SN 2003ma","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Supernova; Gravitational microlensing; Large Magellanic Cloud; Luminosity; Stars; Spectral line; Cosmic dust; Light curve; Interstellar medium","score_opus":0.03133016742429816,"score_gpt":0.2344901555496872,"score_spread":0.20315998812538905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068718676","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9893245,0.0013063485,0.0032899405,0.00058229663,0.000083936604,0.0000056192307,0.00007385273,0.00009912405,0.0052343765],"genre_scores_gemma":[0.99637055,0.0005850434,0.0019184791,0.00026494122,0.00008727655,0.000003694928,0.00009775835,0.000015686102,0.00065657514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999101,0.0000083293135,0.00000565893,0.000024612564,0.000034759,0.000016518643],"domain_scores_gemma":[0.9997944,0.000021506037,0.00006846974,0.000030552255,0.000030951927,0.00005415462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032964165,0.00018025009,0.00016171101,0.0002858017,0.0003535579,0.00090157305,0.0003807075,0.00041610992,0.00034797654],"category_scores_gemma":[0.0005707929,0.00009844979,0.00015804196,0.00021281226,0.00038811102,0.0005195851,0.0006566059,0.0004354543,0.0001797606],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071731384,0.0002050925,0.63066494,0.00014056523,0.0001635363,0.008550278,0.0013166093,0.0016610331,0.20267467,0.018530093,0.0057614734,0.1296143],"study_design_scores_gemma":[0.00006235757,0.00057084166,0.82071763,0.00016529614,0.00013726433,0.020913592,0.0011298547,0.008403065,0.03956079,0.025243947,0.08301172,0.00008368057],"about_ca_topic_score_codex":0.0012091818,"about_ca_topic_score_gemma":0.0025795163,"teacher_disagreement_score":0.0012091818,"about_ca_system_score_codex":0.00026340503,"about_ca_system_score_gemma":0.00023817467,"threshold_uncertainty_score":0.0024043322},"labels":[],"label_agreement":null},{"id":"W2068747194","doi":"10.1088/0004-637x/708/1/675","title":"LONG-TERM MONITORING OF THE DYNAMICS AND PARTICLE ACCELERATION OF KNOTS IN THE JET OF CENTAURUS A","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Physics; Knot (papermaking); Astrophysics; Centaurus A; Particle acceleration; Radio galaxy; Synchrotron; Population; Acceleration; Galaxy; Jet (fluid); Classical mechanics; Mechanics; Nuclear physics","score_opus":0.017028162731801157,"score_gpt":0.2562782708470733,"score_spread":0.23925010811527211,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068747194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99897337,0.0002543973,0.0001685543,0.000015561134,0.000010989978,0.0000043869472,0.00023689968,0.000026602354,0.00030930384],"genre_scores_gemma":[0.9989881,0.000096686905,0.00022929317,0.000012898425,0.000026726793,0.0000069535477,0.00048631072,0.000006759512,0.00014634387],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997092,0.000032622007,0.000025444742,0.000087045366,0.000076944845,0.00006861837],"domain_scores_gemma":[0.9970776,0.00027478175,0.0011068648,0.00030823765,0.0003635264,0.0008691436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006270129,0.00033668452,0.00044480184,0.0038447124,0.00071356754,0.0010433691,0.00055097253,0.00042280584,0.0006762265],"category_scores_gemma":[0.001933326,0.0002282334,0.0003090503,0.001208365,0.0005880217,0.00069050986,0.0013562125,0.0005048814,0.00036220037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042075326,0.00013173517,0.94026667,0.00008350344,0.00020216091,0.00063814945,0.0011549207,0.00040560114,0.039095234,0.00013591327,0.00038660786,0.017078767],"study_design_scores_gemma":[0.000002805222,0.0000645996,0.9988299,0.000005157237,0.000019037418,0.00015776021,0.00009509854,0.00015081187,0.00039554716,0.000029886864,0.00024147844,0.000007879972],"about_ca_topic_score_codex":0.0032414955,"about_ca_topic_score_gemma":0.005004039,"teacher_disagreement_score":0.0038447124,"about_ca_system_score_codex":0.00032532384,"about_ca_system_score_gemma":0.000129363,"threshold_uncertainty_score":0.0064452887},"labels":[],"label_agreement":null},{"id":"W2068764154","doi":"10.1088/0004-637x/764/1/1","title":"X-RAY OBSERVATIONS OF HIGH-B RADIO PULSARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Black-body radiation; Luminosity; Magnetic field; Limit (mathematics); Sigma; Field (mathematics)","score_opus":0.017336347119508055,"score_gpt":0.2873522904972396,"score_spread":0.27001594337773155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068764154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997874,0.00016991736,0.00025931103,0.000030289351,0.000003923348,0.000011661236,0.00016519763,0.000030605035,0.001455075],"genre_scores_gemma":[0.9979365,0.00017429431,0.00089804764,0.000046658635,0.000016480615,0.000011423465,0.00048096123,0.000012478041,0.00042316437],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998914,0.000012721844,0.000009661826,0.000024254758,0.000033367185,0.000028626497],"domain_scores_gemma":[0.99933535,0.00009456373,0.000291411,0.000047040277,0.000075810516,0.00015587892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023297587,0.00026256606,0.00021046042,0.0011986489,0.00040779018,0.0005782187,0.00023856854,0.00023847782,0.00090877706],"category_scores_gemma":[0.00041693085,0.00015091209,0.00013811086,0.0009858435,0.00024207997,0.00020341901,0.0005395583,0.0003439332,0.00038742533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035472322,0.00012694787,0.7893516,0.00010605243,0.00008762156,0.0009841566,0.00033182456,0.0002508006,0.18898615,0.0003149534,0.00083244574,0.018272817],"study_design_scores_gemma":[0.000018420185,0.00012183972,0.99404305,0.000005389295,0.00001769404,0.0006703308,0.00009830618,0.000093305745,0.003555987,0.0000639555,0.0013064304,0.0000052151468],"about_ca_topic_score_codex":0.00099809,"about_ca_topic_score_gemma":0.0018844653,"teacher_disagreement_score":0.0011986489,"about_ca_system_score_codex":0.00017801567,"about_ca_system_score_gemma":0.000103456376,"threshold_uncertainty_score":0.003040135},"labels":[],"label_agreement":null},{"id":"W2068793410","doi":"10.1086/529583","title":"Searching for Dust in the Intracluster Medium from Reddening of Background Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Intracluster medium; Redshift; Galaxy; Astronomy; Galaxy cluster; Extinction (optical mineralogy); Galaxy groups and clusters; Cluster (spacecraft); Galaxy group","score_opus":0.021382372597099863,"score_gpt":0.2454030546732592,"score_spread":0.22402068207615936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068793410","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99832755,0.0001414475,0.0010196392,0.000008717549,0.0000018983246,0.0000051838765,0.00022269673,0.000027584647,0.00024531333],"genre_scores_gemma":[0.99744153,0.00009496309,0.0015258967,0.000007566119,0.0000075819303,0.000003956995,0.00077838654,0.0000055117016,0.00013458647],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996898,0.00003172367,0.000017437433,0.00009642919,0.00010705872,0.000057670186],"domain_scores_gemma":[0.9988979,0.00025791768,0.00037484342,0.00016825667,0.00012650405,0.00017451799],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043420235,0.00027952658,0.00034114913,0.0023136728,0.0004325055,0.0012502624,0.0005567046,0.00029053263,0.00062182144],"category_scores_gemma":[0.0011193906,0.00020984927,0.00032636203,0.0015025559,0.0003470507,0.00038620754,0.00059852184,0.0002195896,0.00027604602],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057801684,0.000033502314,0.9799383,0.000022012231,0.00006216711,0.0001387941,0.000111348214,0.00037921392,0.011144165,0.000109780005,0.00009413508,0.007908816],"study_design_scores_gemma":[0.00000865684,0.000069702335,0.9885449,0.0000053536014,0.00007769824,0.00031386176,0.00014725733,0.0036566881,0.006286015,0.000173136,0.0007080573,0.000008698103],"about_ca_topic_score_codex":0.0032856897,"about_ca_topic_score_gemma":0.0059105977,"teacher_disagreement_score":0.0032856897,"about_ca_system_score_codex":0.00022670464,"about_ca_system_score_gemma":0.00022949775,"threshold_uncertainty_score":0.0065330863},"labels":[],"label_agreement":null},{"id":"W2068813564","doi":"10.1086/528371","title":"Do Broad Absorption Line Quasars Live in Different Environments from Ordinary Quasars?","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Redshift; Astrophysics; Correlation function (quantum field theory); Physics; Autocorrelation; Sky; Cluster analysis; Statistics; Spectral density; Mathematics","score_opus":0.01227778924569687,"score_gpt":0.21556904630624535,"score_spread":0.20329125706054849,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068813564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990477,0.00010243586,0.00014139817,0.00003673202,0.0000017680163,0.0000026961497,0.00005951776,0.000004232192,0.0006034723],"genre_scores_gemma":[0.99947876,0.00009020138,0.00007059585,0.000056594163,0.000009790907,0.0000024398842,0.00016778582,0.0000026405278,0.000121197154],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996076,0.00006745671,0.000019587542,0.00009784679,0.00006494008,0.00014266021],"domain_scores_gemma":[0.99752825,0.0004930569,0.0009555966,0.00024400349,0.00012482629,0.00065419235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050779385,0.00019892633,0.00038455153,0.0014217326,0.00050295336,0.001175017,0.00041669802,0.00037196866,0.002618585],"category_scores_gemma":[0.002172548,0.0001887242,0.00020386909,0.00096742134,0.0012105128,0.0010501978,0.0009923361,0.00031742858,0.00046889024],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013563102,0.000054252487,0.99048936,0.000016896602,0.00005960079,0.000246118,0.00082918967,0.000093649825,0.0022498884,0.000632971,0.0001117064,0.0050806957],"study_design_scores_gemma":[0.000006630254,0.000042515872,0.9980248,0.0000027106516,0.000014285678,0.00022348456,0.00071830396,0.00011406988,0.00011908042,0.0004272885,0.000301553,0.0000052842342],"about_ca_topic_score_codex":0.0026359027,"about_ca_topic_score_gemma":0.0064965556,"teacher_disagreement_score":0.0026359027,"about_ca_system_score_codex":0.00022480484,"about_ca_system_score_gemma":0.00015403594,"threshold_uncertainty_score":0.008760035},"labels":[],"label_agreement":null},{"id":"W2068873867","doi":"10.1086/592820","title":"Information Content in the Galaxy Angular Power Spectrum from the Sloan Digital Sky Survey and Its Implication on Weak-Lensing Analysis","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Spectral density; Sky; Galaxy; Redshift; Multipole expansion; Weak gravitational lensing; Angular spectrum method; Gaussian; Strong gravitational lensing","score_opus":0.01358867258833754,"score_gpt":0.20677391102206477,"score_spread":0.19318523843372723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2068873867","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9734881,0.00030572576,0.020936655,0.0003572841,0.0000067723186,0.000008689711,0.0011703327,0.00011320044,0.0036132885],"genre_scores_gemma":[0.99756145,0.0001385394,0.0015945568,0.000012143665,0.00001482601,0.0000033108759,0.00049385196,0.000008231482,0.00017308394],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996811,0.00006210908,0.000026104512,0.000052083327,0.00012468787,0.00005391239],"domain_scores_gemma":[0.9956571,0.00242404,0.0008307628,0.0004991429,0.0004457312,0.0001433683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00095940224,0.00022380867,0.00020135213,0.0028508678,0.00027565207,0.00086454523,0.00027557742,0.0001641972,0.0018213895],"category_scores_gemma":[0.010065516,0.00011386368,0.00021816426,0.0016532243,0.0008004622,0.0015773358,0.00071054033,0.000274535,0.00023379897],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049765944,0.000097441116,0.67900044,0.00029596343,0.00017693407,0.00088759186,0.0010128003,0.062645376,0.023719253,0.10739382,0.003360244,0.120912395],"study_design_scores_gemma":[0.000018316656,0.000076325516,0.64591265,0.000062114304,0.00006805217,0.00035347263,0.00043587352,0.21773595,0.013198492,0.119789325,0.002260661,0.00008880188],"about_ca_topic_score_codex":0.003407734,"about_ca_topic_score_gemma":0.0020485665,"teacher_disagreement_score":0.003407734,"about_ca_system_score_codex":0.00054546143,"about_ca_system_score_gemma":0.00031056075,"threshold_uncertainty_score":0.0067757964},"labels":[],"label_agreement":null},{"id":"W2069020320","doi":"10.1086/508674","title":"Is There Evidence for Flat Cores in the Halos of Dwarf Galaxies? The Case of NGC 3109 and NGC 6822","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy rotation curve; Dwarf galaxy; Dwarf galaxy problem; Galaxy; Surface brightness; Local Group; Astronomy; Dark matter; Halo; Interacting galaxy","score_opus":0.024592266855726578,"score_gpt":0.2786422668599135,"score_spread":0.2540500000041869,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069020320","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99728084,0.00011239257,0.00096000056,0.000056349847,0.0000015591518,0.000003568175,0.000044029937,0.000019278117,0.0015219373],"genre_scores_gemma":[0.999663,0.000026277054,0.0001728828,0.0000058444903,0.0000013470508,8.0698544e-7,0.000027631953,0.000003055434,0.000099195044],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998871,0.000034714176,0.000005740649,0.000024840825,0.000015869044,0.00003174234],"domain_scores_gemma":[0.99948514,0.00008600402,0.00013787538,0.00011890704,0.000040648752,0.00013147206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037655837,0.00034112652,0.0003150441,0.00035231785,0.0003006427,0.001086425,0.0004547349,0.0003805114,0.0009871682],"category_scores_gemma":[0.0017161955,0.00023153183,0.00029877713,0.00025829536,0.0006106552,0.0005130111,0.000492184,0.00013423698,0.00026179664],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084191177,0.00008254667,0.8488288,0.00015086588,0.00019875723,0.002474369,0.001071763,0.0808255,0.029630102,0.017277204,0.0007644071,0.017853789],"study_design_scores_gemma":[0.00011385851,0.00021587579,0.7826204,0.000054864133,0.00014171287,0.001431895,0.0009255347,0.1885819,0.006030363,0.016719028,0.0030978492,0.000066692286],"about_ca_topic_score_codex":0.012425869,"about_ca_topic_score_gemma":0.011779458,"teacher_disagreement_score":0.012425869,"about_ca_system_score_codex":0.00048803643,"about_ca_system_score_gemma":0.00024223354,"threshold_uncertainty_score":0.024707079},"labels":[],"label_agreement":null},{"id":"W2069070018","doi":"10.1086/422574","title":"Erratum: “The DEEP Groth Strip Survey. VII. The Metallicity of Field Galaxies at 0.26 &lt;<i>z</i>&lt; 0.82 and the Evolution of the Luminosity‐Metallicity Relation” (ApJ, 599, 1006 [2003])","year":2004,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Metallicity; Astrophysics; Galaxy; Luminosity; Galaxy formation and evolution; Astronomy","score_opus":0.010233518289781843,"score_gpt":0.23489299139053293,"score_spread":0.2246594731007511,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069070018","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.003498312,0.0030949216,0.0009798341,0.065978296,0.80654836,0.00012145539,0.08153376,0.0012812144,0.036963854],"genre_scores_gemma":[0.024094684,0.004957776,0.006371912,0.05586274,0.048441462,0.00027537433,0.11499445,0.0016945668,0.74330705],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9986619,0.00012613328,0.00030011538,0.0001871698,0.0006063533,0.00011841837],"domain_scores_gemma":[0.99072695,0.0011732236,0.0007736651,0.0006507555,0.0062313415,0.00044400955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014506122,0.0012940962,0.0010567347,0.0038165564,0.0024468293,0.002424934,0.0019568922,0.0019573225,0.05723034],"category_scores_gemma":[0.012304048,0.0007937718,0.0008736153,0.0028585803,0.00072361145,0.0014349144,0.0013304986,0.0028785602,0.037283946],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022590415,0.000006125734,0.00034099628,0.000031857715,0.000004541939,0.000055528573,0.000009509246,0.000022619926,0.000030360192,0.00014463277,0.9972019,0.0021292402],"study_design_scores_gemma":[0.00005636981,0.000029949713,0.013153568,0.00017869633,0.000047251386,0.00019261408,0.0001482834,0.000112434944,0.00048403066,0.0004984389,0.9850582,0.000040154653],"about_ca_topic_score_codex":0.0814189,"about_ca_topic_score_gemma":0.12992086,"teacher_disagreement_score":0.0814189,"about_ca_system_score_codex":0.0026871304,"about_ca_system_score_gemma":0.0035311044,"threshold_uncertainty_score":0.19145453},"labels":[],"label_agreement":null},{"id":"W2069074368","doi":"10.1086/380439","title":"Geometry of the Large Magellanic Cloud Disk: Results from MACHO and the Two Micron All Sky Survey","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Cepheid variable; Distance modulus; Large Magellanic Cloud; Astrophysics; Light curve; Sky; Photometry (optics); Stellar density; Astronomy; Geometry; Stars","score_opus":0.010574532256327923,"score_gpt":0.22932214780122104,"score_spread":0.2187476155448931,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069074368","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960372,0.00021011068,0.00032535315,0.000016492178,0.0000016453397,0.000004945299,0.0021961685,0.00002114945,0.0011870224],"genre_scores_gemma":[0.9961002,0.000091792426,0.00040033337,0.000006169223,0.000005515398,0.000003565943,0.0032021357,0.00001697369,0.00017332575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968636,0.000059963582,0.000019103287,0.000110572466,0.000072337265,0.000051695388],"domain_scores_gemma":[0.9991837,0.00014467054,0.00026213872,0.00013686139,0.000113304086,0.0001593016],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029961634,0.000365753,0.00032358855,0.0012589433,0.00028249776,0.0005928792,0.00026004904,0.00019553666,0.0009978685],"category_scores_gemma":[0.0010534874,0.00015638222,0.00031373397,0.0014013301,0.00021858423,0.00037567562,0.0006395881,0.00013988289,0.00050411513],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017574859,0.000022793902,0.98042244,0.00003638615,0.00008962135,0.00021741539,0.00025756742,0.0017694612,0.005145856,0.00017969344,0.0006569811,0.011026029],"study_design_scores_gemma":[0.0000024073906,0.000016249507,0.9985304,0.00000200272,0.000012137598,0.000064622676,0.000087087785,0.0005094896,0.00024358589,0.000028759012,0.0004995837,0.0000035889418],"about_ca_topic_score_codex":0.00881522,"about_ca_topic_score_gemma":0.011388569,"teacher_disagreement_score":0.00881522,"about_ca_system_score_codex":0.0003376461,"about_ca_system_score_gemma":0.00015485681,"threshold_uncertainty_score":0.017527819},"labels":[],"label_agreement":null},{"id":"W2069108113","doi":"10.1086/591512","title":"Halo Assembly Bias in Hierarchical Structure Formation","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":269,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Halo; Halo effect; Gaussian; Physics; Statistical physics; Focus (optics); Astrophysics; Galaxy; Quantum mechanics; Optics","score_opus":0.015094146076984167,"score_gpt":0.22306836082074255,"score_spread":0.20797421474375838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069108113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99386865,0.00012416333,0.0047971276,0.00008394423,0.0000032598662,0.000004397994,0.000030719628,0.000047006473,0.001040686],"genre_scores_gemma":[0.999345,0.000030282958,0.0004629348,0.000008145854,0.0000018772074,0.000001986451,0.00001645015,0.000007730218,0.00012562129],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985087,0.00004607705,0.000005831095,0.000026226657,0.00002601147,0.000044992677],"domain_scores_gemma":[0.99735814,0.001212624,0.0006956047,0.00024095415,0.0002178372,0.00027483757],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00084800355,0.00020061014,0.00024659466,0.00050389435,0.00044303387,0.00071175816,0.0003922571,0.00040894168,0.00086017133],"category_scores_gemma":[0.0079249935,0.00019365638,0.00021864612,0.00036612505,0.0007222538,0.0009515936,0.0006992105,0.00028086387,0.00012839829],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032003503,0.00007366149,0.3372611,0.00011492411,0.00013624909,0.0006081984,0.0009943059,0.56805205,0.023949455,0.053717867,0.0011562577,0.013615933],"study_design_scores_gemma":[0.000037785838,0.00008156753,0.0796974,0.000022604867,0.000038854192,0.000167412,0.00016062282,0.8895342,0.0065154717,0.023189299,0.0005100023,0.00004478936],"about_ca_topic_score_codex":0.006007512,"about_ca_topic_score_gemma":0.0058853882,"teacher_disagreement_score":0.006007512,"about_ca_system_score_codex":0.0010489417,"about_ca_system_score_gemma":0.0004072867,"threshold_uncertainty_score":0.011945128},"labels":[],"label_agreement":null},{"id":"W2069273162","doi":"10.1088/0004-637x/774/1/40","title":"GALAXY CLUSTERS IN THE LINE OF SIGHT TO BACKGROUND QUASARS. III. MULTI-OBJECT SPECTROSCOPY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Redshift; Galaxy; Galaxy cluster; Quasar; Spectroscopy; Brightest cluster galaxy; Line-of-sight; Cluster (spacecraft); Interacting galaxy","score_opus":0.013374980407835147,"score_gpt":0.2467445257163837,"score_spread":0.23336954530854856,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069273162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98940533,0.0005932486,0.0024769309,0.00006243612,0.000015572201,0.000022385764,0.0010019338,0.00016103893,0.006261149],"genre_scores_gemma":[0.99644595,0.00012932565,0.0013187921,0.00004499556,0.000015973463,0.000011417395,0.0010000959,0.000009106171,0.0010244307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980396,0.000016683432,0.0000095000505,0.000062508625,0.000044778255,0.00006250851],"domain_scores_gemma":[0.9996418,0.00004650818,0.00014177938,0.000060598144,0.000036063506,0.00007322663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018989279,0.00020072608,0.00018247237,0.001136222,0.00032387493,0.0006182106,0.00030941764,0.00026066517,0.0028731562],"category_scores_gemma":[0.00042152384,0.00013567077,0.00015613415,0.0008143282,0.00013527187,0.0003287378,0.0004344033,0.0001713131,0.0007306851],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031371217,0.00006706675,0.91632336,0.00012337546,0.00011877297,0.00041648353,0.00026870047,0.0017345961,0.043358326,0.001992102,0.0019091959,0.033374224],"study_design_scores_gemma":[0.000005212631,0.000032902768,0.9941968,0.000006106482,0.000020386742,0.00020684075,0.0000730852,0.0011718102,0.001482393,0.00029916616,0.002501796,0.0000034449774],"about_ca_topic_score_codex":0.0023480821,"about_ca_topic_score_gemma":0.0047365376,"teacher_disagreement_score":0.0028731562,"about_ca_system_score_codex":0.00023266998,"about_ca_system_score_gemma":0.00010606263,"threshold_uncertainty_score":0.009611666},"labels":[],"label_agreement":null},{"id":"W2069288948","doi":"10.1086/508152","title":"On the Origin of the Small‐Frequency Spacings Found in the Pulsation Spectra of Hot B Subdwarf Stars","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Asteroseismology; Stars; Subdwarf; Astrophysics; Spectral line; Scale (ratio); Noise (video); Astronomy; White dwarf","score_opus":0.018931388355099166,"score_gpt":0.23778035104740772,"score_spread":0.21884896269230855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069288948","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96713614,0.0009838358,0.028123006,0.00017875303,0.000053950615,0.0000104294995,0.00007318771,0.00012420665,0.003316452],"genre_scores_gemma":[0.9933467,0.00021785777,0.006063982,0.000032868116,0.000038813516,0.0000061952264,0.000056684847,0.00002112163,0.00021572887],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999101,0.000012984117,0.000006967164,0.000037961134,0.000021524469,0.000010422748],"domain_scores_gemma":[0.9986808,0.00071781466,0.00034219836,0.00014880807,0.000058991594,0.00005137307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031072513,0.0002734366,0.00017558645,0.0007571595,0.0003229238,0.00041191306,0.00032032363,0.00040190056,0.0011805749],"category_scores_gemma":[0.002133036,0.000118983866,0.00013129607,0.00043648,0.0007794095,0.00060670887,0.0004658956,0.0004620212,0.00030964427],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011434563,0.00014604352,0.3338906,0.0005012212,0.00007858377,0.0019986005,0.0029377327,0.011032014,0.4633694,0.035599757,0.00071962795,0.1485829],"study_design_scores_gemma":[0.00006468817,0.0005943929,0.8178904,0.00012264728,0.000057987305,0.004780994,0.0012551093,0.03158518,0.068886064,0.06488598,0.009755297,0.00012122984],"about_ca_topic_score_codex":0.000103275604,"about_ca_topic_score_gemma":0.00012006157,"teacher_disagreement_score":0.0011805749,"about_ca_system_score_codex":0.00011111333,"about_ca_system_score_gemma":0.00008165267,"threshold_uncertainty_score":0.0039494634},"labels":[],"label_agreement":null},{"id":"W2069297561","doi":"10.1086/590359","title":"Using<i>Chandra</i>to Unveil the High‐Energy Properties of the High Magnetic Field Radio Pulsar J1119−6127","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Research Canada","funders":"","keywords":"Physics; Pulsar; Astrophysics; Pulsar wind nebula; Neutron star; Astronomy; Black-body radiation; Supernova remnant; Luminosity; Nebula; Binary pulsar; Supernova; Millisecond pulsar; Radiation; Galaxy; Stars; Nuclear physics","score_opus":0.020741514574155132,"score_gpt":0.263554776059922,"score_spread":0.24281326148576687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069297561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91930354,0.0035699098,0.032951698,0.0009495672,0.000475889,0.00016511235,0.0039539123,0.0016290582,0.037001338],"genre_scores_gemma":[0.947176,0.002853423,0.039114967,0.00072797894,0.000359207,0.00010606611,0.004769738,0.00020168912,0.004691032],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99985325,0.000010005584,0.000008953769,0.00004603763,0.000046790894,0.000034897952],"domain_scores_gemma":[0.9995958,0.000042782576,0.0001322424,0.00011528867,0.00004954902,0.0000642354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023665647,0.00032810375,0.00026619754,0.00092747196,0.00049970247,0.001653295,0.0004111534,0.00028713178,0.0020563018],"category_scores_gemma":[0.0005794546,0.00023151992,0.00035372106,0.000651928,0.0004203137,0.0007112161,0.00087288226,0.0008448235,0.00064648816],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003546122,0.00034970455,0.21338949,0.0010051879,0.00026794348,0.0019489513,0.0006511027,0.0016281798,0.5898855,0.0092291245,0.017909484,0.16338077],"study_design_scores_gemma":[0.000121232726,0.00034616812,0.6408343,0.0002057396,0.00027108024,0.00760734,0.00036182711,0.0062008086,0.18755454,0.0044518122,0.15189354,0.00015162447],"about_ca_topic_score_codex":0.0018204916,"about_ca_topic_score_gemma":0.004281281,"teacher_disagreement_score":0.0020563018,"about_ca_system_score_codex":0.0002921461,"about_ca_system_score_gemma":0.00024860527,"threshold_uncertainty_score":0.0068790317},"labels":[],"label_agreement":null},{"id":"W2069578937","doi":"10.1086/309131","title":"The O/H Distribution in NGC 7479: Evidence for a Minor Merger Event","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Spiral galaxy; Galaxy; Extinction (optical mineralogy); H II region; Astronomy; Line (geometry); Star formation","score_opus":0.013023904239500358,"score_gpt":0.25379664578859806,"score_spread":0.2407727415490977,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069578937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99932516,0.00002981739,0.000023183306,0.000009867347,7.0223297e-7,0.0000014161246,0.0000644189,0.0000032560326,0.0005422792],"genre_scores_gemma":[0.99956435,0.000024445457,0.00007188682,0.000010003303,0.0000038052572,0.0000019765998,0.00015093919,0.0000020044536,0.0001705163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983346,0.000011835615,0.0000112756725,0.00003250835,0.000047744135,0.000063071086],"domain_scores_gemma":[0.99955803,0.000044236232,0.00012668704,0.000023916928,0.000081335274,0.00016573607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010572848,0.00021874266,0.00028429288,0.0011848159,0.0009529577,0.0003912993,0.00037223115,0.0003491123,0.001379044],"category_scores_gemma":[0.0005073277,0.000113232,0.00013087559,0.0008495864,0.0005491585,0.00023868596,0.0005393395,0.00015547956,0.00042571817],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021025512,0.000080152335,0.9561224,0.000014648687,0.000039736336,0.0014381978,0.00041627718,0.00022181439,0.036318347,0.00017630143,0.0001651735,0.0047967504],"study_design_scores_gemma":[0.0000032853063,0.000045778932,0.9984518,0.0000013402424,0.000007838861,0.00041716476,0.00021458765,0.00010235758,0.00047352104,0.000025939451,0.00025289232,0.0000033849124],"about_ca_topic_score_codex":0.021035397,"about_ca_topic_score_gemma":0.023544194,"teacher_disagreement_score":0.021035397,"about_ca_system_score_codex":0.00071761454,"about_ca_system_score_gemma":0.00027899857,"threshold_uncertainty_score":0.04182595},"labels":[],"label_agreement":null},{"id":"W2069810205","doi":"10.1088/0004-637x/766/1/3","title":"LIMB-DARKENING COEFFICIENTS FOR ECLIPSING WHITE DWARFS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Limb darkening; White dwarf; Physics; Light curve; Context (archaeology); Astrophysics; Telescope; Large Synoptic Survey Telescope; Stars; Geology","score_opus":0.012873109958202877,"score_gpt":0.23217880663514467,"score_spread":0.2193056966769418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069810205","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89979875,0.00031209175,0.075427644,0.00008421718,0.000016458907,0.000060318085,0.0029863664,0.0016414172,0.019672718],"genre_scores_gemma":[0.982778,0.00016970436,0.01341532,0.000020375915,0.000005358822,0.00002121785,0.0013225642,0.00034428676,0.0019230712],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99991965,0.000013626302,0.000005647377,0.000014335339,0.000027046775,0.000019668187],"domain_scores_gemma":[0.9995608,0.00017650807,0.000054345113,0.00006292149,0.00010554907,0.000039877796],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026458522,0.0002489988,0.00020902992,0.0007603934,0.00033897525,0.00034044785,0.0005258196,0.00022128048,0.0019198295],"category_scores_gemma":[0.0013776236,0.00016084078,0.00055655045,0.0007125937,0.00013065775,0.00031139684,0.00031080158,0.00026772646,0.00054460217],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052365598,0.000039893304,0.082429655,0.00008778322,0.00005848566,0.00013717895,0.00017685008,0.8772935,0.008133191,0.007317863,0.0016202749,0.022652974],"study_design_scores_gemma":[0.000029125398,0.000025108455,0.072125174,0.000021577385,0.000037660026,0.00011514332,0.0000548064,0.9093313,0.008750366,0.0054518906,0.0040183836,0.00003935739],"about_ca_topic_score_codex":0.012997225,"about_ca_topic_score_gemma":0.017030815,"teacher_disagreement_score":0.012997225,"about_ca_system_score_codex":0.0005931465,"about_ca_system_score_gemma":0.000357723,"threshold_uncertainty_score":0.025843143},"labels":[],"label_agreement":null},{"id":"W2069900572","doi":"10.1086/507522","title":"Spectroscopy of Young Planetary Mass Candidates with Disks","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Ophiuchus; Planetary mass; Planet; Planetary system; Stars; Stellar classification; Spectroscopy; T Tauri star","score_opus":0.004077886576251923,"score_gpt":0.20437244568412533,"score_spread":0.20029455910787342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069900572","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99829036,0.00022783804,0.00029796676,0.000020777668,0.0000035655319,0.0000056811978,0.00009557408,0.000020453706,0.0010377719],"genre_scores_gemma":[0.9982722,0.00010112837,0.0007936737,0.000025685615,0.000009206353,0.0000071905743,0.00029503755,0.0000035784046,0.00049228343],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992335,0.000007836934,0.000005153044,0.00002525657,0.000016957265,0.000021475442],"domain_scores_gemma":[0.9997954,0.000037699556,0.00006010467,0.000017168213,0.000026414284,0.00006327731],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002159031,0.00019209192,0.00017584547,0.0010430446,0.0003486822,0.0003782706,0.00025336523,0.00028460365,0.0015586584],"category_scores_gemma":[0.00032619655,0.00010499095,0.00011538469,0.0005859952,0.00010358331,0.00018351106,0.00032690386,0.0001334475,0.00043464563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023485876,0.000066918146,0.8888988,0.000045178927,0.000030058824,0.001212867,0.000380323,0.00008893971,0.097171344,0.00013094666,0.0003712803,0.011368498],"study_design_scores_gemma":[0.000011433727,0.00019685492,0.98408854,0.000008329572,0.000038559436,0.0031258683,0.0004498703,0.00036956335,0.009612109,0.00012886935,0.001964697,0.000005170746],"about_ca_topic_score_codex":0.00036403438,"about_ca_topic_score_gemma":0.00075188937,"teacher_disagreement_score":0.0015586584,"about_ca_system_score_codex":0.00009316245,"about_ca_system_score_gemma":0.000057986334,"threshold_uncertainty_score":0.0052142143},"labels":[],"label_agreement":null},{"id":"W2069955441","doi":"10.1086/382153","title":"<i>Far Ultraviolet Spectroscopic Explorer</i> Observations of G226-29: First Detection of the H <sub>2</sub> Quasi-molecular Satellite at 1150","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; White dwarf; Ultraviolet; Spectral line; Satellite; Astrophysics; Far ultraviolet; Astronomy; Line (geometry); Stars; Optics","score_opus":0.011527724366677232,"score_gpt":0.203968583287811,"score_spread":0.19244085892113377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069955441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966955,0.0002162983,0.00022673575,0.000036901263,0.0000065671506,0.0000053209596,0.0003263746,0.000043429423,0.0024429983],"genre_scores_gemma":[0.9973955,0.00014289889,0.00073421525,0.000048490263,0.000016094888,0.000003926597,0.0008882226,0.000007099836,0.0007635566],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999658,0.0000021265728,0.0000011580537,0.000009161854,0.000012985089,0.000008686703],"domain_scores_gemma":[0.9999033,0.0000059524864,0.000038656093,0.000008876574,0.000008019943,0.000035285837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000042203603,0.00019134553,0.00012007589,0.0003208022,0.00035414065,0.00025462403,0.00022187985,0.0002607283,0.00091543194],"category_scores_gemma":[0.0001125683,0.00009274886,0.00007703114,0.00022580934,0.000235719,0.00018660027,0.00037175257,0.00027962492,0.00035904592],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007392769,0.00021440693,0.4561319,0.00013646456,0.00013814849,0.0032238518,0.00066185236,0.0006667685,0.4997118,0.0008794901,0.003164397,0.034331616],"study_design_scores_gemma":[0.000018702634,0.00033212543,0.9617076,0.000012047149,0.00003677259,0.0019960925,0.00015018167,0.0005367737,0.025774999,0.00022991443,0.009188959,0.000015863397],"about_ca_topic_score_codex":0.0013913773,"about_ca_topic_score_gemma":0.0050522215,"teacher_disagreement_score":0.0013913773,"about_ca_system_score_codex":0.00016236349,"about_ca_system_score_gemma":0.00006822064,"threshold_uncertainty_score":0.003062427},"labels":[],"label_agreement":null},{"id":"W2069964426","doi":"10.1088/0004-637x/768/2/171","title":"GAPS IN THE GD-1 STAR STREAM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"Los Alamos National Laboratory; U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; Chinese Academy of Sciences; Natural Sciences and Engineering Research Council of Canada; Drexel University; Case Western Reserve University; University of Pittsburgh; Johns Hopkins University; Canadian Institute for Advanced Research; Ohio State University; New Mexico State University; University of Portsmouth; Universität Basel; University of Washington; Princeton University","keywords":"Halo; Physics; Astrophysics; Milky Way; Star (game theory); Dark matter; Dark matter halo; Stars; Galaxy","score_opus":0.00617974341932063,"score_gpt":0.20476438429080976,"score_spread":0.19858464087148914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2069964426","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99810565,0.000030804284,0.0009026303,0.000031776082,0.0000035178805,0.0000048635397,0.0001671673,0.000042164174,0.0007113478],"genre_scores_gemma":[0.99862504,0.000019583578,0.0007635871,0.0000110002675,0.0000028107545,0.0000035308594,0.00036451968,0.000016836002,0.00019309211],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988496,0.000013634485,0.0000057489096,0.000036852492,0.000027756185,0.000030983312],"domain_scores_gemma":[0.9991072,0.00028415097,0.00019757319,0.000082536804,0.00014591061,0.00018260807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003232583,0.00019678757,0.00026854864,0.0003629674,0.00032889016,0.0009572282,0.00031857216,0.00026776554,0.0008528559],"category_scores_gemma":[0.0025664603,0.00013732347,0.00021576666,0.0002851882,0.0004225967,0.00044706624,0.00055582606,0.0003143984,0.00014984797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006955601,0.000162759,0.7317259,0.00009577949,0.00009897698,0.0006031288,0.00081314956,0.2037934,0.025521252,0.0150347,0.0029154099,0.018539907],"study_design_scores_gemma":[0.00007131593,0.0002310017,0.4572166,0.00004261491,0.000059711092,0.0002790565,0.00040909785,0.51928645,0.011814331,0.006583328,0.003963999,0.000042505846],"about_ca_topic_score_codex":0.006095661,"about_ca_topic_score_gemma":0.0041661235,"teacher_disagreement_score":0.006095661,"about_ca_system_score_codex":0.0007862902,"about_ca_system_score_gemma":0.00038349666,"threshold_uncertainty_score":0.0121203065},"labels":[],"label_agreement":null},{"id":"W2070014022","doi":"10.1088/0004-637x/732/2/70","title":"LMXB AND IMXB EVOLUTION: I. THE BINARY RADIO PULSAR PSR J1614–2230","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"Science and Technology Facilities Council","keywords":"Physics; Pulsar; Neutron star; Astrophysics; Solar mass; Astronomy; Stars; Orbital period","score_opus":0.017713237708273027,"score_gpt":0.28274282423050134,"score_spread":0.2650295865222283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070014022","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99370897,0.00009998067,0.0033177023,0.000027306516,0.000009598396,0.000019346036,0.00112049,0.00020470769,0.0014918267],"genre_scores_gemma":[0.97640777,0.00011122344,0.017968843,0.000024968645,0.000010836822,0.000055172342,0.004425754,0.00010731095,0.0008880971],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999095,0.000022467222,0.000008689951,0.00002635057,0.000013797016,0.000019076651],"domain_scores_gemma":[0.99977607,0.000075229334,0.000038833954,0.00004984329,0.000032974454,0.000026962187],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002746133,0.00041251825,0.00042538918,0.0004373936,0.00032675712,0.0005130519,0.00051666977,0.00041324875,0.0015125609],"category_scores_gemma":[0.00085305504,0.00027212713,0.0004398054,0.00055907725,0.00019882942,0.0003176729,0.0004131089,0.00039002413,0.00025207014],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001719514,0.00009487195,0.1563244,0.0001013898,0.0001749885,0.00027903507,0.00012571884,0.8172472,0.0034368637,0.0017268605,0.0009995889,0.019317193],"study_design_scores_gemma":[0.000090365545,0.000108059576,0.034526773,0.000014891849,0.000043368902,0.00017345892,0.00008604932,0.95790297,0.0027109887,0.0010014013,0.0033285203,0.00001321038],"about_ca_topic_score_codex":0.009458651,"about_ca_topic_score_gemma":0.011142753,"teacher_disagreement_score":0.009458651,"about_ca_system_score_codex":0.0004361851,"about_ca_system_score_gemma":0.00054032775,"threshold_uncertainty_score":0.018807232},"labels":[],"label_agreement":null},{"id":"W2070014887","doi":"10.1086/422386","title":"The New DAB White Dwarf PG 1603+432 and the DAO/DAB Phenomenon","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; White dwarf; Phenomenon; Astrophysics; Astronomy; Stars","score_opus":0.0072688455068945015,"score_gpt":0.208517641915475,"score_spread":0.2012487964085805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070014887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911739,0.00067171373,0.00024822188,0.00020857455,0.000035031495,0.00000815519,0.00014371352,0.000035900433,0.007474833],"genre_scores_gemma":[0.9984938,0.0001521804,0.00011977307,0.00010700938,0.000035005323,0.0000034078384,0.00018222554,0.000006994478,0.00089962094],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988353,0.000005730411,0.000006675816,0.000036654365,0.000031432315,0.00003597548],"domain_scores_gemma":[0.99985194,0.0000073540778,0.000038102513,0.0000132540645,0.000006564956,0.00008274079],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010342471,0.00021452559,0.00030058483,0.0005741491,0.000710167,0.0006476028,0.0002052743,0.00042541328,0.0015613233],"category_scores_gemma":[0.0002458983,0.00012335363,0.00013697769,0.0005218153,0.0007875357,0.00037042226,0.00086047046,0.00037650147,0.00045565548],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019643006,0.00029936573,0.7871619,0.00021627812,0.00008535698,0.02519056,0.0023722397,0.00016919342,0.108809255,0.011158793,0.005046998,0.057525754],"study_design_scores_gemma":[0.00007711865,0.00020880459,0.9119737,0.00002588295,0.00004367371,0.04628832,0.0011420371,0.0002309097,0.003673664,0.0048563248,0.03146159,0.000017841285],"about_ca_topic_score_codex":0.0025920789,"about_ca_topic_score_gemma":0.0028005608,"teacher_disagreement_score":0.0025920789,"about_ca_system_score_codex":0.00033999115,"about_ca_system_score_gemma":0.00017853922,"threshold_uncertainty_score":0.0052230954},"labels":[],"label_agreement":null},{"id":"W2070039048","doi":"10.1088/0004-637x/790/2/132","title":"SOME LIKE IT HOT: LINKING DIFFUSE X-RAY LUMINOSITY, BARYONIC MASS, AND STAR FORMATION RATE IN COMPACT GROUPS OF GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Star formation; Galaxy; Stellar mass; Galaxy formation and evolution; Stars; Halo; Galaxy group; Star cluster; Galaxy cluster; Galaxy groups and clusters","score_opus":0.008224252178177911,"score_gpt":0.20534372843136298,"score_spread":0.19711947625318507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070039048","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99958926,0.00008478178,0.000031686588,0.0000067484907,5.1717086e-7,0.0000014820961,0.00008865611,0.0000034400302,0.00019355265],"genre_scores_gemma":[0.9996934,0.00002234134,0.000062139465,0.000003629885,0.0000028973461,0.0000010454567,0.00016865568,0.0000020225502,0.000043861186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980205,0.00002662534,0.000015802441,0.000058323207,0.000032744603,0.00006437531],"domain_scores_gemma":[0.9976399,0.00047130487,0.000910622,0.0002038526,0.00015718892,0.000617108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003420814,0.00026056403,0.0002782598,0.0028167514,0.0003351494,0.0008522426,0.00029230103,0.00029887626,0.0012757909],"category_scores_gemma":[0.0019259646,0.00016630562,0.0003071246,0.0012746837,0.00047418577,0.00047137338,0.0010400207,0.00022118365,0.0002811953],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039923296,0.000009751758,0.9982241,0.0000032331318,0.000026300635,0.00001694032,0.00012287406,0.000090353664,0.00039699237,0.000025897625,0.000021392136,0.0010221968],"study_design_scores_gemma":[0.0000019940471,0.000024437108,0.99931455,0.0000027471724,0.00000997814,0.00006265249,0.0002044828,0.0002012189,0.00006424458,0.000036229474,0.00007535053,0.000001958149],"about_ca_topic_score_codex":0.0077715227,"about_ca_topic_score_gemma":0.008177705,"teacher_disagreement_score":0.0077715227,"about_ca_system_score_codex":0.000258254,"about_ca_system_score_gemma":0.00012441706,"threshold_uncertainty_score":0.015452564},"labels":[],"label_agreement":null},{"id":"W2070179115","doi":"10.1088/0004-637x/767/2/164","title":"A PARAMETER-SPACE STUDY OF CARBON-OXYGEN WHITE DWARF MERGERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Toronto","funders":"","keywords":"White dwarf; Physics; Astrophysics; Thermonuclear fusion; Mass ratio; Common envelope; Astronomy; Stars; Plasma; Nuclear physics","score_opus":0.010741449147289436,"score_gpt":0.22673691087818246,"score_spread":0.215995461730893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070179115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99744886,0.000084107494,0.0006506009,0.00006967778,0.000003375371,0.000006796053,0.00007979878,0.000030167617,0.001626628],"genre_scores_gemma":[0.99916995,0.00003512778,0.00045898996,0.0000135087585,0.0000028950865,0.000005244224,0.00012062614,0.000011125383,0.00018255843],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998318,0.000052643976,0.00000670239,0.0000235238,0.000025194742,0.00006023942],"domain_scores_gemma":[0.9986541,0.0008123414,0.00018519799,0.00008845373,0.000097008364,0.00016281859],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053124555,0.00046862056,0.0004419614,0.0011828606,0.0006479541,0.0009536816,0.00072318263,0.0008984935,0.001478882],"category_scores_gemma":[0.0036175237,0.00030171432,0.00065528497,0.0007175263,0.0009659137,0.0008648455,0.00087675505,0.00079881895,0.00009964371],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005109829,0.00020523471,0.037460916,0.000050205123,0.00016926383,0.00065232196,0.0002549337,0.94206655,0.005672971,0.00958566,0.0005520947,0.0028188708],"study_design_scores_gemma":[0.00008200015,0.00012201685,0.010861565,0.0000093418885,0.0000298017,0.00007152718,0.00015645295,0.98533165,0.0009903117,0.0019824319,0.00034356993,0.000019374978],"about_ca_topic_score_codex":0.010337545,"about_ca_topic_score_gemma":0.00520044,"teacher_disagreement_score":0.010337545,"about_ca_system_score_codex":0.0007463408,"about_ca_system_score_gemma":0.00041825126,"threshold_uncertainty_score":0.020554721},"labels":[],"label_agreement":null},{"id":"W2070279464","doi":"10.1088/0004-637x/694/1/704","title":"ERRATUM: “THE 5.25 AND 5.7 μm ASTRONOMICAL POLYCYCLIC AROMATIC HYDROCARBON EMISSION FEATURES” (2009, ApJ, 690, 1208)","year":2009,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Atomic and Molecular Physics","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Overtone; Spectral line; Physics; Population; Chemistry; Crystallography; Computational chemistry; Astronomy","score_opus":0.0048773822992091275,"score_gpt":0.218048373037396,"score_spread":0.21317099073818688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070279464","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0019659018,0.0025246798,0.001181912,0.04730239,0.9314377,0.000055623183,0.0014105046,0.0006535161,0.013467777],"genre_scores_gemma":[0.041846212,0.011577662,0.009886394,0.11967805,0.2843437,0.00027778107,0.008964181,0.0022606316,0.5211653],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99933076,0.00007712697,0.00012987878,0.00015306628,0.00025086058,0.0000582901],"domain_scores_gemma":[0.9967404,0.00045373305,0.000332835,0.00031888267,0.0019328939,0.00022131961],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010671447,0.0020972406,0.00088085094,0.0022286389,0.0039182575,0.0021328086,0.0020855702,0.0039275126,0.04471856],"category_scores_gemma":[0.00833527,0.0008904142,0.0010351263,0.0015628447,0.0015866455,0.0027868475,0.0014286885,0.0061613633,0.042557754],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005329988,0.00002133611,0.0004078442,0.000096296266,0.000014774076,0.00031098543,0.000033203774,0.000042454547,0.00025865601,0.00065343187,0.9895175,0.008590299],"study_design_scores_gemma":[0.000050001512,0.000070338,0.004816642,0.00019805595,0.000044761648,0.00084633264,0.00025767492,0.00027775348,0.0009959254,0.0011927934,0.99119407,0.000055590917],"about_ca_topic_score_codex":0.010264362,"about_ca_topic_score_gemma":0.010783758,"teacher_disagreement_score":0.04471856,"about_ca_system_score_codex":0.0017270771,"about_ca_system_score_gemma":0.0019182978,"threshold_uncertainty_score":0.14959848},"labels":[],"label_agreement":null},{"id":"W2070289033","doi":"10.1086/506137","title":"Rates and Properties of Type Ia Supernovae as a Function of Mass and Star Formation in Their Host Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":559,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"Supernova; Star formation; Galaxy; Initial mass function; Star (game theory); Type (biology); Function (biology)","score_opus":0.010591504866565496,"score_gpt":0.20616995182119932,"score_spread":0.19557844695463383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070289033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973525,0.0006739341,0.00006977697,0.00005074766,0.0000035025168,0.00000456718,0.0010092632,0.000018227893,0.00081752625],"genre_scores_gemma":[0.99782,0.00042407057,0.000055729466,0.000013894577,0.000012726121,0.00000460968,0.001069121,0.0000069554926,0.0005928542],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998031,0.000045699464,0.000024425168,0.000049087692,0.000030624105,0.000047011203],"domain_scores_gemma":[0.9944607,0.0021598893,0.0017776061,0.00046398235,0.00040390703,0.0007338698],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081844267,0.00015452302,0.00023664994,0.0014038888,0.00015916182,0.00090252666,0.00027280953,0.00046502642,0.0022205748],"category_scores_gemma":[0.0041133366,0.00024358073,0.0003575885,0.00079994486,0.00029058885,0.00046262058,0.0003645614,0.0003581436,0.0007801965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013609062,0.000019626385,0.9954554,0.000009751829,0.00005863051,0.000046392095,0.00008678756,0.00034754013,0.00065048726,0.000090991445,0.00031358283,0.0027847367],"study_design_scores_gemma":[0.0000035035896,0.000026417607,0.9992424,0.0000034539555,0.000014924966,0.00017029159,0.000044177752,0.00019825113,0.00009538055,0.000038564798,0.00015914848,0.0000035136209],"about_ca_topic_score_codex":0.0041854503,"about_ca_topic_score_gemma":0.0039729453,"teacher_disagreement_score":0.0041854503,"about_ca_system_score_codex":0.00023646565,"about_ca_system_score_gemma":0.00009949141,"threshold_uncertainty_score":0.008322179},"labels":[],"label_agreement":null},{"id":"W2070357585","doi":"10.1086/518551","title":"Thermalization in Relativistic Outflows and the Correlation between Spectral Hardness and Apparent Luminosity in Gamma‐Ray Bursts","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":152,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Lorentz factor; Astrophysics; Gamma-ray burst; Photosphere; Poynting vector; Luminosity; Jet (fluid); Spectral energy distribution; Compton scattering; RADIUS; Radiation; Electron; Lorentz transformation; Astronomy; Spectral line; Nuclear physics; Galaxy","score_opus":0.010429324457965477,"score_gpt":0.23332424925875506,"score_spread":0.22289492480078957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070357585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998852,0.00013560631,0.0005726399,0.000016926275,0.0000015408485,0.0000013759094,0.000027751823,0.000012217891,0.00037995478],"genre_scores_gemma":[0.999696,0.00004541951,0.00012144706,0.0000066956472,0.000008040412,0.0000012130919,0.000041299005,0.0000033647384,0.000076546414],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992144,0.000019685562,0.000009122964,0.00002104967,0.000012049459,0.000016613669],"domain_scores_gemma":[0.9976617,0.00075442437,0.001101753,0.00022775105,0.00008995508,0.00016444281],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035811713,0.00022758522,0.00016548921,0.0008081625,0.00013027247,0.0008825669,0.00028486864,0.0003034764,0.0012564085],"category_scores_gemma":[0.0023019833,0.00024050364,0.00015504312,0.00054297986,0.000553939,0.00042819863,0.00042326917,0.00025659974,0.00022080017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039798874,0.00004289505,0.9799487,0.000019374052,0.000036556517,0.00024195322,0.00025698106,0.0017878376,0.011178995,0.0004713785,0.000045494024,0.00557186],"study_design_scores_gemma":[0.0000075860544,0.00005804973,0.9956655,0.0000030700517,0.00001788843,0.00029431542,0.00008147584,0.0023565867,0.00087881193,0.0005480543,0.00008065389,0.0000080611635],"about_ca_topic_score_codex":0.0005027151,"about_ca_topic_score_gemma":0.00037051004,"teacher_disagreement_score":0.0012564085,"about_ca_system_score_codex":0.00016128906,"about_ca_system_score_gemma":0.00006155878,"threshold_uncertainty_score":0.004203081},"labels":[],"label_agreement":null},{"id":"W2070376208","doi":"10.1086/503157","title":"The Origin of Structures in Wolf-Rayet Winds: <i>FUSE</i> Observations of WR 135","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Université de Montréal","funders":"","keywords":"Absorption (acoustics); Dispersion (optics); Rest (music); Rest frame; Space (punctuation); Velocity dispersion","score_opus":0.014047704330408492,"score_gpt":0.24102434362002031,"score_spread":0.22697663928961181,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070376208","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99931324,0.00006406176,0.00012596602,0.000007068045,0.0000011681392,0.0000020404152,0.00009601936,0.000010683743,0.00037983726],"genre_scores_gemma":[0.999684,0.000016027112,0.00014323113,0.0000040639957,0.0000011630026,9.3398114e-7,0.00009630419,0.0000017526048,0.000052562755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999465,0.0000022009972,0.0000033422193,0.000016913486,0.000015793288,0.000015387204],"domain_scores_gemma":[0.9998271,0.000007459913,0.00010312785,0.000012983088,0.000013388625,0.00003604519],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000070984395,0.00018836716,0.0001064517,0.00036054812,0.00025351698,0.000506733,0.00022528529,0.00022210866,0.0004120918],"category_scores_gemma":[0.00026497376,0.00012936053,0.000117408235,0.00028760138,0.0002148941,0.00020790451,0.00038133425,0.00025410648,0.00012445288],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027288456,0.00007658804,0.6284372,0.00007607215,0.00010100294,0.0009427762,0.0007325202,0.0009449251,0.354926,0.0007161877,0.00034217033,0.012431688],"study_design_scores_gemma":[0.000010792798,0.00009817602,0.98764473,0.000006189968,0.000030484654,0.00068763975,0.00018209619,0.0006416529,0.009834518,0.000102941376,0.0007525156,0.000008067853],"about_ca_topic_score_codex":0.0058070617,"about_ca_topic_score_gemma":0.007831764,"teacher_disagreement_score":0.0058070617,"about_ca_system_score_codex":0.00031444276,"about_ca_system_score_gemma":0.000107560336,"threshold_uncertainty_score":0.011546552},"labels":[],"label_agreement":null},{"id":"W2070424195","doi":"10.1086/526396","title":"Wide‐Field Survey of Globular Clusters in M31. II. Kinematics of the Globular Cluster System","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Physics; Rotation (mathematics); Astrophysics; Halo; Galaxy rotation curve; Velocity dispersion; Cluster (spacecraft); Galaxy; Geometry","score_opus":0.013611311413610607,"score_gpt":0.2170934739700284,"score_spread":0.2034821625564178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070424195","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99802977,0.00014103066,0.00011273535,0.000027913644,0.0000010511778,0.000010495946,0.0009279262,0.000013027358,0.00073602964],"genre_scores_gemma":[0.9943698,0.00016491543,0.00067737565,0.000024577916,0.000008126469,0.000015576661,0.003932529,0.000005416571,0.00080152915],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981505,0.000017401753,0.000009352808,0.00005046378,0.00004763733,0.00006011325],"domain_scores_gemma":[0.9994623,0.00003156377,0.00014457709,0.000056314453,0.0001049475,0.00020027682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026270153,0.00019766617,0.00013603219,0.0017563776,0.0005491093,0.00023883778,0.00023200805,0.00020615438,0.0010043613],"category_scores_gemma":[0.00041069268,0.00009696827,0.00016632068,0.0014651066,0.00016919718,0.00025347833,0.00071783824,0.00013171013,0.00064102036],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052033876,0.000027070302,0.9783934,0.000018750996,0.0000211869,0.00016251339,0.00035486152,0.0003000872,0.00833898,0.00013856392,0.00091653236,0.01127604],"study_design_scores_gemma":[8.794737e-7,0.000013391937,0.9989058,0.000001772105,0.0000017794735,0.00006337186,0.00006101594,0.00010202503,0.0001311491,0.000014906796,0.0007023518,0.0000015960516],"about_ca_topic_score_codex":0.01656815,"about_ca_topic_score_gemma":0.031669885,"teacher_disagreement_score":0.01656815,"about_ca_system_score_codex":0.00037156855,"about_ca_system_score_gemma":0.00043424105,"threshold_uncertainty_score":0.032943428},"labels":[],"label_agreement":null},{"id":"W2070426978","doi":"10.1086/507865","title":"Formation and Collapse of Nonaxisymmetric Protostellar Cores in Planar Magnetic Interstellar Clouds: Formulation of the Problem and Linear Analysis","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Dimensionless quantity; Instability; Gravitational collapse; Ambipolar diffusion; Molecular cloud; Magnetohydrodynamics; Supercritical fluid; Dispersion (optics); Planar","score_opus":0.006314859377381448,"score_gpt":0.21237357303480625,"score_spread":0.2060587136574248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070426978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.77947575,0.0015741561,0.1996141,0.0013210272,0.00005971997,0.0001746333,0.0003638112,0.00012194822,0.01729484],"genre_scores_gemma":[0.98319465,0.0005591697,0.010355064,0.00007180456,0.00007876733,0.0001463104,0.00014538046,0.000033029133,0.0054157474],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999038,0.000023737835,0.0000037190803,0.000017544227,0.000026922873,0.000024228724],"domain_scores_gemma":[0.9997603,0.000108515276,0.00006879552,0.000008267141,0.000032468415,0.000021680135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024866263,0.00064657046,0.00035073422,0.00042046158,0.00048548752,0.00092426006,0.00086916453,0.00080045266,0.0010912967],"category_scores_gemma":[0.0012763707,0.00030597896,0.0005083353,0.000267728,0.0010139748,0.0005133137,0.00081526575,0.00043337798,0.00010927722],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003375336,0.000037136455,0.0020777418,0.00009462473,0.000020835238,0.0002370527,0.0000708108,0.9651683,0.003580683,0.0257112,0.0002742516,0.0026936035],"study_design_scores_gemma":[0.000010140712,0.0000276911,0.00062240905,0.000004701988,0.0000042532793,0.00002988958,0.000033802826,0.99403703,0.00043064522,0.004558819,0.00023647411,0.000004168421],"about_ca_topic_score_codex":0.012226719,"about_ca_topic_score_gemma":0.0056370236,"teacher_disagreement_score":0.012226719,"about_ca_system_score_codex":0.0013622366,"about_ca_system_score_gemma":0.0008532156,"threshold_uncertainty_score":0.024311125},"labels":[],"label_agreement":null},{"id":"W2070644994","doi":"10.1088/0004-637x/759/1/27","title":"GLOBAL OPTIMIZATION METHODS FOR GRAVITATIONAL LENS SYSTEMS WITH REGULARIZED SOURCES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Regularization (linguistics); Deconvolution; Degrees of freedom (physics and chemistry); Lens (geology); Estimator; Source code; Optimization problem; Algorithm; Mathematical optimization; Blind deconvolution; Inverse problem; Computer science; Mathematics; Applied mathematics; Optics; Physics; Artificial intelligence; Mathematical analysis; Statistics","score_opus":0.01956574941466421,"score_gpt":0.2930210144801717,"score_spread":0.2734552650655075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070644994","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0037272298,0.00013424427,0.9949917,0.00009572373,0.000009779391,0.000021261138,0.000028936747,0.00014414536,0.00084698014],"genre_scores_gemma":[0.22390915,0.00036263146,0.76938075,0.00017756535,0.00007416199,0.0004647443,0.0003057657,0.00052548596,0.0047998023],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99945074,0.00027858818,0.00002404173,0.000098057375,0.000107133805,0.000041378986],"domain_scores_gemma":[0.9976574,0.0016046929,0.00025611662,0.00012987689,0.00028252898,0.000069235255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002341959,0.0016077467,0.0013464919,0.0012742868,0.0005539736,0.0010389908,0.001443169,0.0019541737,0.002070015],"category_scores_gemma":[0.0043957974,0.00090929423,0.0012537051,0.00076259975,0.0015491484,0.0011190024,0.0016735459,0.0016266481,0.000482375],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000010509078,0.000009517095,0.00014644436,0.000024837804,0.000025879994,0.00001535121,0.000023125893,0.9837382,0.0003398651,0.009630121,0.0002256257,0.0058105234],"study_design_scores_gemma":[0.0000027075755,0.0000042510032,0.00001875471,0.0000026736845,0.0000017260053,0.0000026005644,0.0000024358294,0.9953903,0.00008704297,0.004315709,0.00016912805,0.0000026136174],"about_ca_topic_score_codex":0.005665842,"about_ca_topic_score_gemma":0.0049517294,"teacher_disagreement_score":0.005665842,"about_ca_system_score_codex":0.0011348801,"about_ca_system_score_gemma":0.00133105,"threshold_uncertainty_score":0.012385607},"labels":[],"label_agreement":null},{"id":"W2070734907","doi":"10.1088/0004-637x/767/2/101","title":"A NEW MILKY WAY HALO STAR CLUSTER IN THE SOUTHERN GALACTIC SKY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Centre National de la Recherche Scientifique; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; York University; Office of Science; Johns Hopkins University; Science and Technology Facilities Council; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Milky Way; Globular cluster; Astronomy; Stellar population; Absolute magnitude; Surface brightness; Star cluster; Luminosity; Horizontal branch; Luminosity function; Galactic halo; Stars; Population; Galaxy; Halo; Star formation","score_opus":0.009945223212321497,"score_gpt":0.21233580176944164,"score_spread":0.20239057855712014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070734907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986858,0.0003463993,0.00017707367,0.000034011635,0.000008604147,0.000004687917,0.00007382732,0.000021969889,0.000647784],"genre_scores_gemma":[0.9981488,0.0001866974,0.0005285839,0.000027508628,0.000024090323,0.000003570671,0.00039627915,0.0000052000096,0.0006792999],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989045,0.000006103664,0.0000045625043,0.00003215778,0.000039816226,0.000026976999],"domain_scores_gemma":[0.9996755,0.000015752867,0.00006811903,0.00003593704,0.00004162373,0.00016305025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012532317,0.00018343897,0.00024230954,0.0006992689,0.00066144654,0.00069647486,0.00035509773,0.00025944403,0.0007548627],"category_scores_gemma":[0.00026345174,0.000117609714,0.00018199938,0.00077645906,0.00035346946,0.00026054514,0.0011703098,0.00017369827,0.00027064682],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003624309,0.0000630088,0.9131177,0.00013974888,0.000105483356,0.009471872,0.001832785,0.0004971821,0.047431592,0.0012021622,0.0008708065,0.024905188],"study_design_scores_gemma":[0.000023438084,0.00028238457,0.9682934,0.000022257133,0.000066781686,0.008614088,0.0008997057,0.0010511376,0.005558479,0.0005343016,0.014626607,0.000027428117],"about_ca_topic_score_codex":0.0031768838,"about_ca_topic_score_gemma":0.00642011,"teacher_disagreement_score":0.0031768838,"about_ca_system_score_codex":0.00038557992,"about_ca_system_score_gemma":0.00027767968,"threshold_uncertainty_score":0.0063168406},"labels":[],"label_agreement":null},{"id":"W2070886716","doi":"10.1086/518109","title":"A Study of the 3.3 and 3.4 μm Emission Features in Proto–Planetary Nebulae","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Nebula; Planetary nebula; Stars; Spectral line; Reflection nebula; Star (game theory); Emission spectrum; Astronomy","score_opus":0.008258488781349894,"score_gpt":0.24825698137612978,"score_spread":0.2399984925947799,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070886716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980026,0.00025595585,0.0006910459,0.000012829381,0.0000023188918,0.0000061738947,0.00010298533,0.000020770709,0.0009053643],"genre_scores_gemma":[0.9981483,0.00007574034,0.001283748,0.000019617566,0.0000043721393,0.000010186596,0.00021893151,0.000007994881,0.00023102397],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.0000046689124,0.0000028249926,0.000021193286,0.000025905363,0.000016483136],"domain_scores_gemma":[0.9997749,0.00003266524,0.000087733664,0.000022044118,0.00003160449,0.000051146737],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013343108,0.00018228611,0.00016307349,0.0006578596,0.00036727867,0.00028432894,0.0002760368,0.000268405,0.00048076833],"category_scores_gemma":[0.0002862462,0.00018280516,0.00033140468,0.00043574686,0.00023055222,0.00022270261,0.00025927243,0.0003898106,0.0001652601],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028990288,0.000063253094,0.22423598,0.000080846956,0.00007011315,0.00069575664,0.0004273642,0.00040098384,0.7583102,0.00023166608,0.00016437224,0.015029443],"study_design_scores_gemma":[0.0000042348224,0.00004813246,0.9867312,0.0000040079394,0.000012427065,0.00076802616,0.00006282184,0.00039747328,0.011288204,0.00007636618,0.00060092384,0.0000062498466],"about_ca_topic_score_codex":0.0013527502,"about_ca_topic_score_gemma":0.0017289007,"teacher_disagreement_score":0.0013527502,"about_ca_system_score_codex":0.00022782922,"about_ca_system_score_gemma":0.00010149154,"threshold_uncertainty_score":0.0026897192},"labels":[],"label_agreement":null},{"id":"W2070924920","doi":"10.1086/429814","title":"An<i>RXTE</i>Archival Search for Coherent X‐Ray Pulsations in the Low‐Mass X‐Ray Binary 4U 1820−30","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Binary number; Globular cluster; X-ray binary; Millisecond; Modulation (music); Range (aeronautics); Binary star; Phase (matter); Coherence (philosophical gambling strategy)","score_opus":0.020399670578503448,"score_gpt":0.2796559112610981,"score_spread":0.2592562406825947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070924920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99522346,0.00013694426,0.0019221347,0.000036858957,0.000003858149,0.00004371891,0.0011075751,0.0000887199,0.0014367698],"genre_scores_gemma":[0.96832687,0.0001539351,0.022126686,0.00011717871,0.000034483644,0.000106063446,0.0070841694,0.00007404817,0.0019765294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973637,0.000041409206,0.000022511264,0.000083660394,0.00007216435,0.000043777407],"domain_scores_gemma":[0.99926156,0.00010907313,0.00024617263,0.00013376262,0.00009078521,0.00015856554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007098253,0.00026881968,0.00032495437,0.0018478895,0.00080994994,0.00089616666,0.00041991423,0.00035163213,0.0012422269],"category_scores_gemma":[0.00092955143,0.00027870134,0.00031254964,0.0011401518,0.0002114954,0.00035414926,0.0009617273,0.00034059232,0.00041138704],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076712563,0.0004970578,0.72506404,0.00020375491,0.00032047415,0.0007127308,0.00083997863,0.002452531,0.1988925,0.0007653105,0.0034802188,0.06600429],"study_design_scores_gemma":[0.00009101495,0.00045123542,0.96507484,0.000021198199,0.00016306779,0.0006993912,0.00026890208,0.004548507,0.020931853,0.00026662578,0.0074532353,0.000030193001],"about_ca_topic_score_codex":0.0024286024,"about_ca_topic_score_gemma":0.009895003,"teacher_disagreement_score":0.0024286024,"about_ca_system_score_codex":0.00024795075,"about_ca_system_score_gemma":0.0003859622,"threshold_uncertainty_score":0.00482893},"labels":[],"label_agreement":null},{"id":"W2070944459","doi":"10.1086/381495","title":"X‐Ray Reflection from Inhomogeneous Accretion Disks. I. Toy Models and Photon Bubbles","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Reflection (computer programming); Spectral line; Accretion (finance); Photon; Ionization; Line (geometry); Slab; Radiation; Constant (computer programming)","score_opus":0.019912309042418863,"score_gpt":0.24508952464051698,"score_spread":0.2251772155980981,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070944459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9742181,0.00044447955,0.018711839,0.00026846686,0.000018711351,0.00003390703,0.00027015683,0.00018275228,0.005851708],"genre_scores_gemma":[0.9954072,0.0001409493,0.0035388588,0.00003923072,0.000010317643,0.000033654585,0.00013512162,0.000041459338,0.0006532155],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998066,0.00007743527,0.000012381752,0.000030282963,0.00004050021,0.00003284123],"domain_scores_gemma":[0.99899584,0.00048786763,0.00025345443,0.00009475996,0.00006644517,0.00010163003],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039412206,0.0006653157,0.0005485624,0.00043347754,0.00039348967,0.00094638113,0.001091568,0.0010542696,0.001142307],"category_scores_gemma":[0.0023209113,0.0004431887,0.0007460294,0.00034914806,0.0010051482,0.00082341244,0.00083170773,0.00064440625,0.00016611036],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017202675,0.000059138598,0.005160618,0.00008994695,0.000045416185,0.00040640205,0.00014865627,0.9738599,0.0073540555,0.011311417,0.00023799921,0.0011544336],"study_design_scores_gemma":[0.00005551354,0.000042133153,0.0010565976,0.0000084717785,0.000010869298,0.000081778024,0.000035613164,0.9946518,0.0010744742,0.0028112822,0.00016080927,0.000010564545],"about_ca_topic_score_codex":0.0040447144,"about_ca_topic_score_gemma":0.00088892353,"teacher_disagreement_score":0.0040447144,"about_ca_system_score_codex":0.0009125067,"about_ca_system_score_gemma":0.00023928499,"threshold_uncertainty_score":0.0080423355},"labels":[],"label_agreement":null},{"id":"W2070944674","doi":"10.1086/378719","title":"<i>Far Ultraviolet Spectroscopic Explorer</i>Observation of the Ultramassive White Dwarf PG 1658+441","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Balmer series; White dwarf; Far ultraviolet; Physics; Astrophysics; Ultraviolet; Spectral line; Satellite; Emission spectrum; Astronomy; Stars; Optics","score_opus":0.013711257302968913,"score_gpt":0.2199631065418895,"score_spread":0.2062518492389206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2070944674","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99405235,0.00023973832,0.0003165068,0.00006039734,0.0000058304017,0.000007669124,0.0012520683,0.00007331554,0.00399215],"genre_scores_gemma":[0.99502146,0.00016195643,0.0008132388,0.00005642652,0.000021468868,0.0000052344226,0.0028338924,0.000010798417,0.0010755805],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999579,0.0000030310996,0.0000012671861,0.000009328007,0.000015296959,0.000013101988],"domain_scores_gemma":[0.99991286,0.000007630413,0.000033235978,0.000007523837,0.000009812166,0.00002895423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000065559594,0.00021456364,0.00012326121,0.0010629593,0.00034830646,0.00027061123,0.00016363422,0.00020544934,0.0012305916],"category_scores_gemma":[0.00009020534,0.00008971261,0.00015711863,0.00041363025,0.000107651555,0.0001782844,0.00028476137,0.0001489495,0.00029388652],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010374753,0.00036692328,0.5171368,0.00017780838,0.00023733496,0.0032350435,0.0004771291,0.002528617,0.41663957,0.0012584291,0.0041559883,0.052748848],"study_design_scores_gemma":[0.000016965289,0.00013387432,0.98469514,0.0000068827767,0.00004539965,0.0009863185,0.00006448014,0.0006523754,0.00959665,0.0002057562,0.0035827295,0.00001353933],"about_ca_topic_score_codex":0.002629602,"about_ca_topic_score_gemma":0.005079733,"teacher_disagreement_score":0.002629602,"about_ca_system_score_codex":0.00015522269,"about_ca_system_score_gemma":0.00006591133,"threshold_uncertainty_score":0.0052285194},"labels":[],"label_agreement":null},{"id":"W2071062897","doi":"10.1086/510609","title":"The Fragmenting Superbubble Associated with the H<scp>ii</scp>Region W4","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of New Brunswick; University of Manitoba","funders":"","keywords":"Superbubble; Physics; Astrophysics; Halo; Galaxy; Polarization (electrochemistry); Line-of-sight; Cluster (spacecraft); Milky Way; Astronomy; Interstellar medium; Chemistry","score_opus":0.008806157159081595,"score_gpt":0.21746941778047554,"score_spread":0.20866326062139395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071062897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99796045,0.000029896037,0.0003586808,0.00001135204,0.0000017712165,0.0000032831165,0.00006826949,0.000019856947,0.0015464305],"genre_scores_gemma":[0.99899405,0.000010267882,0.0003464147,0.0000066802663,0.0000029585126,0.0000018467996,0.00020042865,0.0000045282486,0.00043279625],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994755,0.0000020618663,0.0000014895293,0.000014986863,0.000011871718,0.000022021091],"domain_scores_gemma":[0.9998431,0.000011741787,0.000053108142,0.000017885246,0.00002066116,0.00005340969],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004142616,0.00013322169,0.00010453261,0.00050452346,0.00035440509,0.00029423504,0.00024388585,0.00015078881,0.0020439762],"category_scores_gemma":[0.00015268852,0.00012025808,0.00012508249,0.00029998305,0.00027174366,0.00017787467,0.00046356747,0.00016744553,0.00023638946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053779304,0.00003857893,0.49944764,0.00007278911,0.000082950544,0.0037840058,0.00051803165,0.0009436384,0.47047344,0.000900439,0.0010088941,0.022191744],"study_design_scores_gemma":[0.000007637372,0.00004249352,0.98413914,0.000005416415,0.00001569317,0.00122409,0.0001953975,0.0011960146,0.010822969,0.00020943189,0.0021353653,0.0000062751387],"about_ca_topic_score_codex":0.005358864,"about_ca_topic_score_gemma":0.0056628264,"teacher_disagreement_score":0.005358864,"about_ca_system_score_codex":0.00029538854,"about_ca_system_score_gemma":0.00013216719,"threshold_uncertainty_score":0.0106553435},"labels":[],"label_agreement":null},{"id":"W2071082264","doi":"10.1086/499224","title":"An Extreme Case of a Misaligned Highly Flattened Wind in the Wolf‐Rayet Binary CX Cephei","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; Astrophysics; Wolf–Rayet star; Stars; Polarization (electrochemistry); Orbital plane; Orbital period; Orbital inclination; Linear polarization; Asymmetry; Mass ratio; Binary number; Optics","score_opus":0.013393341945540708,"score_gpt":0.23095777713247992,"score_spread":0.21756443518693921,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071082264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99628913,0.000056264133,0.0027642578,0.00004751612,0.000010149178,0.000004021229,0.000060461523,0.000024933697,0.00074328855],"genre_scores_gemma":[0.99881244,0.0000198775,0.00092868396,0.000009025336,0.0000050964954,0.0000016382119,0.000058336813,0.0000035768123,0.000161254],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984336,0.00001895111,0.000013247279,0.000048451402,0.000031035965,0.000044961544],"domain_scores_gemma":[0.9997645,0.000040516356,0.000097377466,0.0000400402,0.000014246442,0.000043278505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020660718,0.00022258758,0.00028247808,0.00030727603,0.00047617397,0.0007850631,0.0001951208,0.00058803294,0.0011387022],"category_scores_gemma":[0.0010611184,0.0001724842,0.000109428,0.0002758069,0.00036150613,0.00034626992,0.00041347768,0.00028586574,0.00029505638],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001238544,0.00012791649,0.7321722,0.00010119461,0.00010666552,0.02885474,0.000536909,0.028358653,0.17203434,0.011224989,0.0012212379,0.024022603],"study_design_scores_gemma":[0.00009301646,0.00043497077,0.8141526,0.000042429197,0.0001074174,0.03171302,0.0011452296,0.094778016,0.04123419,0.009543643,0.006674808,0.000080693506],"about_ca_topic_score_codex":0.0011641918,"about_ca_topic_score_gemma":0.002046537,"teacher_disagreement_score":0.0011641918,"about_ca_system_score_codex":0.00016777604,"about_ca_system_score_gemma":0.00013267834,"threshold_uncertainty_score":0.0038093925},"labels":[],"label_agreement":null},{"id":"W2071085980","doi":"10.1086/322316","title":"The Halo White Dwarf WD 0346+246 Revisited","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Opacity; Halo; Helium; Astrophysics; Physics; Hydrogen; Interstellar medium; Astronomy; Atomic physics; Stars; Optics; Quantum mechanics","score_opus":0.010479095842920533,"score_gpt":0.22703475607034884,"score_spread":0.2165556602274283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071085980","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97105956,0.009940851,0.002132014,0.0013096518,0.00026095897,0.0000065231498,0.00015051512,0.0001150117,0.0150248585],"genre_scores_gemma":[0.9936667,0.001968296,0.0006171173,0.00022667578,0.000120680634,0.0000015251243,0.00010499775,0.000028238557,0.003265727],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999199,0.000009316867,0.00000353873,0.00001660178,0.000027639082,0.000022951679],"domain_scores_gemma":[0.9999175,0.000007267601,0.000018019524,0.000012657962,0.000013815614,0.00003073315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002130301,0.00026843036,0.000283318,0.00048434304,0.00063329167,0.0010043842,0.000333975,0.0004436509,0.00092044385],"category_scores_gemma":[0.00032308022,0.00009702118,0.00027939468,0.0003739626,0.00048923254,0.00032244512,0.0009113086,0.0004163125,0.00038140843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014424791,0.0000773586,0.35815746,0.0010223564,0.0004933328,0.02773871,0.0019034217,0.012527421,0.24758297,0.086932346,0.014816691,0.24730538],"study_design_scores_gemma":[0.00012570781,0.0003376738,0.5509132,0.00023112167,0.0003449478,0.029146574,0.0026484437,0.014868195,0.05423525,0.064822644,0.2821968,0.00012942737],"about_ca_topic_score_codex":0.0078962715,"about_ca_topic_score_gemma":0.0061567076,"teacher_disagreement_score":0.0078962715,"about_ca_system_score_codex":0.0006905872,"about_ca_system_score_gemma":0.00037678765,"threshold_uncertainty_score":0.015700638},"labels":[],"label_agreement":null},{"id":"W2071111798","doi":"10.1086/375267","title":"SN 1979C VLBI: 22 Years of Almost Free Expansion","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Ejecta; Astrophysics; Very-long-baseline interferometry; Supernova; Light curve; Kinetic energy; Astronomy","score_opus":0.009846237741316646,"score_gpt":0.2221787677114371,"score_spread":0.21233252997012045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071111798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9723502,0.0015268915,0.002254215,0.00023344735,0.000071565024,0.000056752324,0.00583106,0.00031706868,0.017358802],"genre_scores_gemma":[0.98792297,0.00023054187,0.0008010054,0.00021053547,0.00006204861,0.000054063483,0.0069808294,0.00008151751,0.003656493],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981123,0.0000087419685,0.0000068242302,0.000053729687,0.000051633204,0.00006794329],"domain_scores_gemma":[0.9996382,0.000029058792,0.00010711927,0.0000460297,0.00006019692,0.00011933857],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034105615,0.00036947618,0.0004451507,0.00082432857,0.00062748435,0.000642065,0.0006092846,0.00057768635,0.0024455017],"category_scores_gemma":[0.00079360884,0.00021322741,0.00032806623,0.0005120919,0.0002312706,0.00022965467,0.0006161183,0.00055046735,0.0014880069],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012977446,0.000245314,0.8155714,0.00027380724,0.00064688886,0.0032654926,0.00031074867,0.0039744703,0.114953175,0.005170169,0.012895957,0.04139488],"study_design_scores_gemma":[0.000034367476,0.000078745696,0.97842807,0.000021064108,0.00006835063,0.0018429492,0.000035366927,0.0019881781,0.0034672539,0.000360743,0.013648522,0.000026489792],"about_ca_topic_score_codex":0.016914865,"about_ca_topic_score_gemma":0.021867458,"teacher_disagreement_score":0.016914865,"about_ca_system_score_codex":0.0011999736,"about_ca_system_score_gemma":0.0003488328,"threshold_uncertainty_score":0.033632815},"labels":[],"label_agreement":null},{"id":"W2071165683","doi":"10.1086/591314","title":"The Progenitors of Type Ia Supernovae","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Victoria","funders":"","keywords":"Supernova; White dwarf; Stars; Galaxy; Star formation; Stellar evolution; Degenerate energy levels","score_opus":0.01426135657606122,"score_gpt":0.23982564781026722,"score_spread":0.225564291234206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071165683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96133506,0.0052401177,0.02026769,0.00018007917,0.000111846006,0.000036936013,0.00052348286,0.00019604461,0.012108642],"genre_scores_gemma":[0.9856399,0.0024858306,0.004769846,0.00009075083,0.000042084488,0.000015866677,0.0009542454,0.000022253322,0.0059792222],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99985707,0.00001790953,0.000017219354,0.000045185167,0.00003456375,0.000028130911],"domain_scores_gemma":[0.99949336,0.000110252,0.00011825662,0.00008420863,0.00007054143,0.0001233254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037615027,0.0002676984,0.0003282408,0.00046412673,0.00039502652,0.0012693168,0.0004182302,0.00043776463,0.0011928503],"category_scores_gemma":[0.0011584669,0.00030555687,0.00020837624,0.00044222228,0.00029831805,0.0005080807,0.0007014755,0.0006308339,0.0010642031],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000308773,0.0001585733,0.5563597,0.0003175762,0.00014466849,0.003081395,0.0007478391,0.0046426044,0.26899037,0.07632859,0.0022073104,0.08671255],"study_design_scores_gemma":[0.000090120884,0.00053062796,0.53098416,0.00028035505,0.00019816247,0.029415896,0.0014459,0.021955546,0.1629453,0.085561566,0.16651039,0.000081923776],"about_ca_topic_score_codex":0.00066412694,"about_ca_topic_score_gemma":0.0006460518,"teacher_disagreement_score":0.0012693168,"about_ca_system_score_codex":0.00045318657,"about_ca_system_score_gemma":0.00033796104,"threshold_uncertainty_score":0.0039904118},"labels":[],"label_agreement":null},{"id":"W2071256685","doi":"10.1086/518957","title":"Revealing the Galactic H<scp>ii</scp>Region G84.9+0.5 through 5 GHz Continuum and Polarization Emission and a Voigt Profile Analysis of Radio Recombination Line Observations","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Calgary; Brandon University","funders":"","keywords":"Physics; Astrophysics; Outflow; Nebula; Line (geometry); Emission spectrum; Spectral line; Ionization; Polarization (electrochemistry); Supernova remnant; Photoionization; Supernova; Atomic physics; Astronomy; Stars; Ion","score_opus":0.020057713584743515,"score_gpt":0.2575913104184981,"score_spread":0.23753359683375458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071256685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98954636,0.0001798985,0.00097088196,0.0002654993,0.000034527733,0.000023324965,0.0012736724,0.00021292309,0.0074929027],"genre_scores_gemma":[0.99256307,0.00009084967,0.0012771534,0.00006119914,0.000039795214,0.00000604957,0.0019460617,0.000050016977,0.0039658523],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989426,0.000007354031,0.000004131517,0.000032845488,0.000033654684,0.000027690796],"domain_scores_gemma":[0.99976,0.00002192941,0.000058618407,0.000021887037,0.0000692141,0.000068367684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015191465,0.00012331331,0.00011151934,0.0010101012,0.00035812464,0.0004470631,0.00024130224,0.00033044713,0.009310783],"category_scores_gemma":[0.00037664597,0.00014019829,0.00015498976,0.00061236636,0.00012188055,0.00026226157,0.00023889063,0.00012519823,0.0014975136],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074382167,0.0001090658,0.4502869,0.0002465876,0.00009780027,0.0017250334,0.00043175914,0.0007265013,0.4694846,0.00082065177,0.015229451,0.060097884],"study_design_scores_gemma":[0.000020571524,0.00005458894,0.9803931,0.000012457737,0.000027941009,0.00045480812,0.00018242047,0.0006002119,0.012482599,0.00012661022,0.0056380876,0.0000065445506],"about_ca_topic_score_codex":0.001928565,"about_ca_topic_score_gemma":0.0056028054,"teacher_disagreement_score":0.009310783,"about_ca_system_score_codex":0.00011830517,"about_ca_system_score_gemma":0.00013852262,"threshold_uncertainty_score":0.031147659},"labels":[],"label_agreement":null},{"id":"W2071296189","doi":"10.1086/376518","title":"The Incidence of Strong‐Lensing Clusters in the Red‐Sequence Cluster Survey","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cluster (spacecraft); Astrophysics; Physics; Cosmology; Redshift; Galaxy cluster; Weak gravitational lensing; Population; Gravitational lens; Substructure; Lens (geology); Galaxy; Sequence (biology); Optics; Demography; Chemistry","score_opus":0.018289741630690505,"score_gpt":0.2460069944217081,"score_spread":0.2277172527910176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071296189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978721,0.0002020813,0.000104547355,0.00006206241,0.0000038512776,0.0000030382553,0.00042820166,0.000013547179,0.0013105095],"genre_scores_gemma":[0.9992786,0.00015040897,0.00006536587,0.000013009049,0.00000465575,0.0000012251251,0.000317303,0.0000020235937,0.0001674471],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992842,0.00013163556,0.000068773836,0.0001612279,0.0002387352,0.00011546639],"domain_scores_gemma":[0.9972349,0.00047690063,0.001233992,0.00026233072,0.0003342343,0.00045769362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000659587,0.00011180416,0.00012614421,0.0015114481,0.00029115402,0.00047000608,0.00026687476,0.0001722574,0.0016946944],"category_scores_gemma":[0.0019887602,0.00015348803,0.00017298391,0.0010258963,0.00043570824,0.0003172498,0.00076054013,0.00022589722,0.00017631525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024710882,0.0000027364338,0.9963599,0.000010029792,0.000020026793,0.00003915813,0.00011160317,0.00007654203,0.000537323,0.00013987656,0.00025624613,0.0024218215],"study_design_scores_gemma":[6.5413906e-7,0.000010104819,0.9991208,0.000002839002,0.000006213613,0.00015674632,0.00016104679,0.00007083313,0.0001767298,0.000019586612,0.0002727296,0.0000017840337],"about_ca_topic_score_codex":0.01604299,"about_ca_topic_score_gemma":0.030820485,"teacher_disagreement_score":0.01604299,"about_ca_system_score_codex":0.0004519915,"about_ca_system_score_gemma":0.0004302051,"threshold_uncertainty_score":0.031899214},"labels":[],"label_agreement":null},{"id":"W2071297720","doi":"10.1088/0004-637x/721/2/1184","title":"ECCENTRICITY TRAP: TRAPPING OF RESONANTLY INTERACTING PLANETS NEAR THE DISK INNER EDGE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Planet; Physics; Eccentricity (behavior); Protoplanetary disk; Trapping; Astrophysics; Planetary system; Planetary migration; Enhanced Data Rates for GSM Evolution; Astronomy","score_opus":0.010451275770036399,"score_gpt":0.2410777988913474,"score_spread":0.230626523121311,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071297720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91333765,0.00033660923,0.08165792,0.000097008655,0.000015851396,0.000019348996,0.000015606105,0.00014468217,0.0043753195],"genre_scores_gemma":[0.9952867,0.000028965536,0.0040833876,0.000008335076,0.000002136305,0.000003993078,0.0000055056516,0.000006086185,0.00057485735],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999409,0.0000065500544,0.0000020429216,0.000015723828,0.000013453329,0.000021402948],"domain_scores_gemma":[0.9997297,0.00006699032,0.000094099494,0.000033734774,0.000034619487,0.00004086543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014477427,0.00014014028,0.00019285738,0.00020467682,0.00041166908,0.0002739125,0.0004622082,0.00023937147,0.0013017649],"category_scores_gemma":[0.0006769355,0.00013249426,0.00011827652,0.00006133617,0.00041179275,0.0005291896,0.00066676934,0.0002173968,0.00016439318],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004792495,0.000109666,0.0319494,0.00028039256,0.000079200516,0.0021764922,0.0011484062,0.07447953,0.7802129,0.06263088,0.0007131072,0.045740694],"study_design_scores_gemma":[0.000083265964,0.0005182653,0.013130193,0.000028554408,0.00005141343,0.0029064466,0.00034051543,0.7588572,0.2005685,0.019923434,0.0035298732,0.000062259634],"about_ca_topic_score_codex":0.00038535084,"about_ca_topic_score_gemma":0.00035770697,"teacher_disagreement_score":0.0013017649,"about_ca_system_score_codex":0.00016492512,"about_ca_system_score_gemma":0.00015924394,"threshold_uncertainty_score":0.0043548346},"labels":[],"label_agreement":null},{"id":"W2071316062","doi":"10.1088/0004-637x/728/1/52","title":"INTERGALACTIC TRANSMISSION AND ITS IMPACT ON THE Lyα LINE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":190,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Ontario Tech University","funders":"","keywords":"Intergalactic travel; Redshift; Cosmic microwave background; Galaxy; Reionization; Spectral line; Optical depth; Photon; Background radiation; Line (geometry)","score_opus":0.014318924550589291,"score_gpt":0.23495561423214223,"score_spread":0.22063668968155295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071316062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997424,0.00010004007,0.0012656815,0.000028111048,0.0000023197765,0.0000028967436,0.00008818467,0.000029673662,0.0010590979],"genre_scores_gemma":[0.99934274,0.000059029735,0.00036512953,0.0000040645577,0.0000018331145,0.000001450402,0.000070899274,0.0000126871255,0.00014227652],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99986887,0.00004875462,0.0000033794133,0.00002045813,0.000020112586,0.0000384554],"domain_scores_gemma":[0.9990839,0.00044937528,0.00023567808,0.0000818448,0.00007730686,0.000071888455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003001945,0.00051779166,0.00020593002,0.00051889144,0.00022781795,0.0005406396,0.0007308255,0.0005032279,0.0014998157],"category_scores_gemma":[0.0019709002,0.00022340487,0.0004142249,0.0006066042,0.0003175306,0.000565495,0.0005295807,0.00041215008,0.00017250114],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021297047,0.00011239893,0.09785624,0.00004191614,0.00010361392,0.0005087615,0.00013023405,0.8825644,0.012236044,0.0017053593,0.00010919582,0.0044188714],"study_design_scores_gemma":[0.000071314804,0.00025706246,0.09109445,0.000019394203,0.00008986204,0.00018222183,0.00016162815,0.8955851,0.010822972,0.0011484277,0.0005330358,0.000034649594],"about_ca_topic_score_codex":0.007040779,"about_ca_topic_score_gemma":0.0033714636,"teacher_disagreement_score":0.007040779,"about_ca_system_score_codex":0.00054686517,"about_ca_system_score_gemma":0.0001611461,"threshold_uncertainty_score":0.013999581},"labels":[],"label_agreement":null},{"id":"W2071536872","doi":"10.1086/377195","title":"The Secular Evolution of the Primordial Kuiper Belt","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Apsidal precession; Planet; Planetary system; Planetary migration; Mechanical wave; Longitudinal wave; Caustic (mathematics); Astrophysics; Classical mechanics; Wave propagation","score_opus":0.0035021619720511364,"score_gpt":0.183105197041943,"score_spread":0.17960303506989186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071536872","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9245217,0.0002977407,0.059851766,0.00037301364,0.000031769217,0.000033516597,0.0003893443,0.00048215393,0.01401904],"genre_scores_gemma":[0.98922485,0.000106383464,0.008239869,0.000035903136,0.000012319138,0.000022025566,0.00017283905,0.00004671385,0.0021392037],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999441,0.000015262183,0.000002134424,0.000012790471,0.000011057528,0.000014594686],"domain_scores_gemma":[0.9998258,0.000055628505,0.000035481644,0.00002150495,0.000025821691,0.000035781697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020556142,0.00039297855,0.00033299418,0.00027242565,0.00045644728,0.00095974194,0.00078119227,0.00068658125,0.0013800162],"category_scores_gemma":[0.001352767,0.00031019768,0.00033821666,0.0002427364,0.0006596335,0.0008131496,0.0005439133,0.00042969198,0.00017077081],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000355491,0.000019660516,0.00635938,0.000013146609,0.000016907516,0.00010862255,0.00007115453,0.97575945,0.0011346316,0.01431412,0.00031168183,0.0018557159],"study_design_scores_gemma":[0.00000936237,0.000009406402,0.00061977224,0.0000011035097,0.0000027575552,0.000012801504,0.000009017211,0.9974546,0.0001323126,0.0014264368,0.00031990244,0.0000026193673],"about_ca_topic_score_codex":0.026004376,"about_ca_topic_score_gemma":0.0081943525,"teacher_disagreement_score":0.026004376,"about_ca_system_score_codex":0.0011285018,"about_ca_system_score_gemma":0.00080906565,"threshold_uncertainty_score":0.051706016},"labels":[],"label_agreement":null},{"id":"W2071568436","doi":"10.1088/0004-637x/802/1/28","title":"NEAR-INFRARED THERMAL EMISSION DETECTIONS OF A NUMBER OF HOT JUPITERS AND THE SYSTEMATICS OF GROUND-BASED NEAR-INFRARED PHOTOMETRY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"York University; Université de Montréal","funders":"Centre National de la Recherche Scientifique","keywords":"Hot Jupiter; Photometry (optics); Eclipse; Asteroid; Light curve; Gas giant; Ephemeris; Thermal emission","score_opus":0.014417922216362813,"score_gpt":0.24223870658596028,"score_spread":0.22782078436959746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071568436","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99726945,0.0002607532,0.0011101036,0.00002145725,0.000005307892,0.000009709708,0.0003559602,0.00008451882,0.000882718],"genre_scores_gemma":[0.9982534,0.000053349442,0.0009968458,0.000015482665,0.000010776364,0.000010025365,0.00051147083,0.000021469143,0.00012703627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989152,0.00016207805,0.0000754232,0.00039899023,0.00033889565,0.00010951116],"domain_scores_gemma":[0.995223,0.0012898751,0.0018064863,0.00088600174,0.00053622545,0.0002583665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00091102684,0.00031050955,0.00032566892,0.0017356665,0.00038182936,0.0006264691,0.00047431618,0.00028160872,0.0004990584],"category_scores_gemma":[0.004200909,0.00030877552,0.00025862508,0.0010584621,0.00036592424,0.00033354576,0.00066211884,0.0002880962,0.00017485734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008272059,0.000019379715,0.97475475,0.000023512786,0.00012916354,0.00008054186,0.00026750934,0.00084966514,0.011997326,0.00007913883,0.0002045389,0.011511761],"study_design_scores_gemma":[0.0000032097807,0.000014683658,0.9972262,0.00000476197,0.000030456633,0.00010386572,0.00003901374,0.0010753901,0.0012253602,0.000045132296,0.00022743549,0.000004474664],"about_ca_topic_score_codex":0.008421052,"about_ca_topic_score_gemma":0.017093062,"teacher_disagreement_score":0.008421052,"about_ca_system_score_codex":0.0003886214,"about_ca_system_score_gemma":0.0001284289,"threshold_uncertainty_score":0.016744077},"labels":[],"label_agreement":null},{"id":"W2071655161","doi":"10.1086/497109","title":"A 2.1<i>M</i><sub>⊙</sub>Pulsar Measured by Relativistic Orbital Decay","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":283,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Pulsar; Binary pulsar; Neutron star; Millisecond pulsar; Astrophysics; Orbital period; White dwarf; Astronomy; Gravitational wave; X-ray pulsar; Orbital decay; Pulsar planet; Stars; Satellite","score_opus":0.010541276747388336,"score_gpt":0.2805665244757984,"score_spread":0.27002524772841,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071655161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99410313,0.00012670044,0.0014573323,0.00004795098,0.000012837728,0.000010597972,0.0002941755,0.000084583444,0.0038626697],"genre_scores_gemma":[0.99686426,0.00005759456,0.0021332875,0.000029369332,0.000014521385,0.00000860682,0.0005575667,0.000014977145,0.00031973934],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989116,0.000013391526,0.00000861095,0.000025918198,0.0000428327,0.00001808704],"domain_scores_gemma":[0.99972266,0.000044313365,0.00012445508,0.000035842037,0.00003793802,0.000034863453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029960892,0.00018844871,0.00016474468,0.00047823528,0.00033698286,0.00039014203,0.00023979085,0.00028184993,0.00072504545],"category_scores_gemma":[0.0007915568,0.00010329323,0.000093721144,0.00041900654,0.00034000754,0.0002727409,0.0003779761,0.00029511465,0.00025494467],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061418343,0.00015580925,0.6335472,0.00012659834,0.000065355576,0.0009762338,0.00037064616,0.0008183612,0.3278523,0.005356523,0.0017951699,0.02832171],"study_design_scores_gemma":[0.000030883606,0.00042002928,0.8882829,0.000013890586,0.00007720891,0.0030991093,0.00013670676,0.0045745373,0.09540793,0.0012365954,0.006694351,0.000025907832],"about_ca_topic_score_codex":0.0006070114,"about_ca_topic_score_gemma":0.00085534796,"teacher_disagreement_score":0.00072504545,"about_ca_system_score_codex":0.00019242152,"about_ca_system_score_gemma":0.00011963873,"threshold_uncertainty_score":0.0024254918},"labels":[],"label_agreement":null},{"id":"W2071810769","doi":"10.1086/421288","title":"The Evolution of Gravitationally Unstable Protoplanetary Disks: Fragmentation and Possible Giant Planet Formation","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":213,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Protoplanetary disk; Formation and evolution of the Solar System; Adiabatic process; Equation of state; Planet; Smoothed-particle hydrodynamics; Protoplanet; Thick disk; Gravitational collapse; Thermodynamics","score_opus":0.0058676637366788425,"score_gpt":0.2191654901818202,"score_spread":0.21329782644514134,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071810769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99854666,0.000050333423,0.0006664316,0.00004810784,0.000002406156,0.0000061983924,0.00014056363,0.00003836944,0.0005009887],"genre_scores_gemma":[0.9985661,0.000044172702,0.0010095916,0.000018346367,0.0000036978645,0.000009815327,0.00022361729,0.000016658612,0.00010790905],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991024,0.00002110946,0.000005182043,0.00001886931,0.000017349967,0.000027303866],"domain_scores_gemma":[0.99935275,0.00031401357,0.00009801729,0.000056655066,0.00004228181,0.00013621246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028195477,0.0005331872,0.00049193844,0.00046614412,0.0006999373,0.00084778666,0.0012814587,0.0011172913,0.0006226567],"category_scores_gemma":[0.0018679634,0.00037559954,0.0006904454,0.0005089263,0.00085504603,0.0006032067,0.0005384298,0.00072870986,0.000094498835],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000121429905,0.00014040821,0.040315494,0.00003439605,0.00012941723,0.0004792776,0.00015004489,0.95113033,0.004503863,0.0012853637,0.0002114548,0.0014984984],"study_design_scores_gemma":[0.00008147971,0.000082951046,0.015793221,0.0000052168025,0.000027190237,0.00011305467,0.00008015676,0.98144126,0.0012134324,0.0009503499,0.0001976055,0.000014045676],"about_ca_topic_score_codex":0.018726964,"about_ca_topic_score_gemma":0.008984593,"teacher_disagreement_score":0.018726964,"about_ca_system_score_codex":0.0011318749,"about_ca_system_score_gemma":0.0005803071,"threshold_uncertainty_score":0.037235916},"labels":[],"label_agreement":null},{"id":"W2071853857","doi":"10.1088/0004-637x/770/1/47","title":"CONSTRAINING PRIMORDIAL MAGNETIC FIELDS THROUGH LARGE-SCALE STRUCTURE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Laurentian University","funders":"","keywords":"Cosmic microwave background; Magnetic field; Big Bang nucleosynthesis; Faraday effect; Dynamo; Cosmology; Amplitude; Universe; Cosmic background radiation; Halo","score_opus":0.005391594786114442,"score_gpt":0.22979709513690608,"score_spread":0.22440550035079163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071853857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91523695,0.0036965297,0.06840209,0.00031208067,0.000029058088,0.000014116367,0.000333957,0.00022823634,0.011747027],"genre_scores_gemma":[0.99265504,0.00078182895,0.0058571803,0.000033475735,0.000042866046,0.0000077390905,0.00026400632,0.000022870154,0.00033500488],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999044,0.000025619733,0.000004293938,0.000031910313,0.000017346754,0.000016324419],"domain_scores_gemma":[0.99882895,0.00049903087,0.00039635313,0.00015035894,0.000036702128,0.00008865587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045447162,0.0005088557,0.00033171254,0.0007079699,0.00033403776,0.00065305206,0.0005471947,0.00039921064,0.0006066476],"category_scores_gemma":[0.0023927984,0.00027344987,0.00025809498,0.0005040142,0.0005287608,0.00094777386,0.0008942837,0.0004011935,0.00017881983],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003574974,0.00018831083,0.38846695,0.0007330636,0.00056422636,0.0012573269,0.00061667484,0.23243341,0.14216335,0.13736361,0.001986702,0.093868874],"study_design_scores_gemma":[0.000080530575,0.00018515703,0.30885285,0.00007801303,0.00017620792,0.00037602815,0.00009784345,0.51483333,0.018890154,0.14654514,0.0097964555,0.000088337634],"about_ca_topic_score_codex":0.0014408873,"about_ca_topic_score_gemma":0.0019583148,"teacher_disagreement_score":0.0014408873,"about_ca_system_score_codex":0.00032303095,"about_ca_system_score_gemma":0.00015468858,"threshold_uncertainty_score":0.0028650165},"labels":[],"label_agreement":null},{"id":"W2071856498","doi":"10.1088/0004-637x/774/1/33","title":"X-RAY OBSERVATIONS OF THE SUPERNOVA REMNANT CTB 87 (G74.9+1.2): AN EVOLVED PULSAR WIND NEBULA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Manitoba","funders":"","keywords":"Physics; Nebula; Astrophysics; Pulsar wind nebula; Supernova remnant; Pulsar; Emission nebula; Astronomy; Point source; Protoplanetary nebula; Supernova; Stars; Optics","score_opus":0.016514755708824835,"score_gpt":0.22037615282193534,"score_spread":0.20386139711311052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071856498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982432,0.000117030315,0.000108188084,0.000022784086,0.0000045856114,0.000009431397,0.00030858326,0.000028406112,0.0011577242],"genre_scores_gemma":[0.99727577,0.00014332446,0.0007850357,0.000037404432,0.000015456619,0.0000069846064,0.001093747,0.000016026623,0.0006263329],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995136,0.0000022882887,0.000002419193,0.000009487408,0.000020650928,0.000013895576],"domain_scores_gemma":[0.999864,0.000008205793,0.000036507965,0.000011328152,0.00002278735,0.00005722547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006143211,0.00020148637,0.00021827745,0.00075169845,0.0004108076,0.00028971827,0.00021814948,0.00022595085,0.0007421722],"category_scores_gemma":[0.00012703589,0.00010927743,0.00012412187,0.00053951767,0.00024324075,0.00011517935,0.00032679198,0.00029095533,0.00028967272],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067109696,0.00043151752,0.5949675,0.00014865259,0.00014989337,0.008719995,0.00059163274,0.00095308415,0.35626897,0.0005843582,0.0036905129,0.032822765],"study_design_scores_gemma":[0.000010826775,0.00008641878,0.9913067,0.0000056704953,0.00002003819,0.0022637618,0.00007344023,0.0003776565,0.0040022186,0.000030120269,0.0018183966,0.0000046970804],"about_ca_topic_score_codex":0.0065844706,"about_ca_topic_score_gemma":0.017096164,"teacher_disagreement_score":0.0065844706,"about_ca_system_score_codex":0.00025550436,"about_ca_system_score_gemma":0.00016030169,"threshold_uncertainty_score":0.013092279},"labels":[],"label_agreement":null},{"id":"W2071921359","doi":"10.1088/0004-637x/783/1/60","title":"SYNTHETIC OBSERVATIONS OF THE EVOLUTION OF STARLESS CORES IN A MOLECULAR CLOUD SIMULATION: COMPARISONS WITH JCMT DATA AND PREDICTIONS FOR ALMA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Molecular cloud; Order (exchange); Star formation; Protostar; Core (optical fiber); Cloud computing","score_opus":0.026450736814260332,"score_gpt":0.26176125522626764,"score_spread":0.2353105184120073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2071921359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989843,0.000013039283,0.0003844812,0.000038122926,0.0000041165417,0.000008021227,0.0002184722,0.000027998703,0.0003214523],"genre_scores_gemma":[0.99883896,0.000009812056,0.00066747185,0.00001070641,0.00000294433,0.000005698878,0.00041871742,0.000007679927,0.000038032667],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998647,0.00003316864,0.000011266093,0.000033579345,0.000025037529,0.00003222679],"domain_scores_gemma":[0.9989864,0.00034490423,0.00020484441,0.00014747426,0.00013396092,0.00018242172],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043118862,0.00030099752,0.00020967567,0.00040034385,0.00030764128,0.00046740889,0.00058302894,0.00047085786,0.00038302768],"category_scores_gemma":[0.0020649207,0.00018984481,0.0003517604,0.00035831536,0.0004119378,0.00031080542,0.00031215747,0.0003804931,0.000053437136],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094354735,0.0006889516,0.33393747,0.000067338464,0.00024828527,0.00052526616,0.0003454112,0.6234625,0.029605828,0.003810159,0.0012274572,0.0051378435],"study_design_scores_gemma":[0.00010459915,0.0001374492,0.09492205,0.0000061564688,0.000024576582,0.000058319718,0.00008606217,0.90110123,0.0026859483,0.00055089244,0.00030367036,0.00001910164],"about_ca_topic_score_codex":0.010146836,"about_ca_topic_score_gemma":0.008123952,"teacher_disagreement_score":0.010146836,"about_ca_system_score_codex":0.00073231664,"about_ca_system_score_gemma":0.00034938278,"threshold_uncertainty_score":0.020175517},"labels":[],"label_agreement":null},{"id":"W2072080672","doi":"10.1088/0004-637x/783/2/69","title":"X-RAY OBSERVATIONS OF BLACK WIDOW PULSARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Millisecond pulsar; Pulsar; Orbital elements; Orbital period; Binary star; Spectral line; Neutron star; Solar mass; Binary number; Flux (metallurgy)","score_opus":0.01984362592467466,"score_gpt":0.3034466149103891,"score_spread":0.28360298898571445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072080672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980868,0.00015184558,0.0003431903,0.000017089389,0.000008345703,0.000011369308,0.00022032004,0.00002240378,0.0011386783],"genre_scores_gemma":[0.9967085,0.00014241585,0.0011623682,0.00004508934,0.000013178066,0.000010619172,0.00071714725,0.0000093546705,0.0011912484],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990594,0.0000064998776,0.000009181475,0.000017318647,0.000024569168,0.000036552137],"domain_scores_gemma":[0.9998091,0.000020910336,0.000060151488,0.000019423702,0.000021336202,0.00006907901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014656455,0.0002152269,0.00015389544,0.00059783313,0.00042369444,0.00043314337,0.00019105857,0.00018673412,0.0012965136],"category_scores_gemma":[0.0003317287,0.00013402823,0.00013168476,0.00043713851,0.00014616358,0.00027475785,0.0004985328,0.00029845798,0.0002546677],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010768188,0.0002320738,0.80322224,0.00010018955,0.00010715507,0.0016301852,0.0015866887,0.00028117164,0.12765875,0.000691984,0.0016801757,0.061732594],"study_design_scores_gemma":[0.000046527504,0.0007371693,0.96426654,0.000016232594,0.00003601249,0.0016995894,0.0004707724,0.00048623094,0.019208396,0.00021746373,0.012796725,0.000018384366],"about_ca_topic_score_codex":0.0014570882,"about_ca_topic_score_gemma":0.0044476492,"teacher_disagreement_score":0.0014570882,"about_ca_system_score_codex":0.000134343,"about_ca_system_score_gemma":0.00008318974,"threshold_uncertainty_score":0.004337311},"labels":[],"label_agreement":null},{"id":"W2072145316","doi":"10.1088/0004-637x/743/2/138","title":"A SPECTROSCOPIC SURVEY AND ANALYSIS OF BRIGHT, HYDROGEN-RICH WHITE DWARFS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":351,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Balmer series; Instability strip; Astrophysics; Stars; Physics; Spectral line; Brown dwarf; Stellar classification; Degenerate energy levels; Binary number; Astronomy; Emission spectrum; Mathematics","score_opus":0.018842669350652944,"score_gpt":0.2295664183809231,"score_spread":0.21072374903027014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072145316","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979424,0.00014863141,0.0006663498,0.000021924305,0.0000017382557,0.000014412824,0.00056058366,0.000025915735,0.0006180515],"genre_scores_gemma":[0.9925168,0.00025478136,0.0036309753,0.0000441105,0.000018053759,0.000017812974,0.0027164267,0.000017373277,0.0007835942],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995352,0.000078480894,0.00005117194,0.0001374071,0.00012848196,0.00006932648],"domain_scores_gemma":[0.99819607,0.0001964793,0.00045437706,0.00025159103,0.00047846872,0.00042311483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009304357,0.0002591874,0.00024008597,0.0032176815,0.0005080134,0.00044566792,0.0003306192,0.00015829533,0.00046475895],"category_scores_gemma":[0.0013700083,0.00016337434,0.00014220184,0.0018908961,0.00025426134,0.0003615563,0.00069030136,0.00018862724,0.00035489537],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002983102,0.000041472475,0.97593486,0.000023484523,0.000019953837,0.000092421666,0.0005655906,0.00014629489,0.010201825,0.00009476943,0.00020846442,0.012640999],"study_design_scores_gemma":[0.0000026029368,0.000041713134,0.997308,0.0000037275677,0.000008766242,0.00013998138,0.00016231205,0.00024385472,0.0011638907,0.000022164415,0.00090031273,0.000002766474],"about_ca_topic_score_codex":0.01086751,"about_ca_topic_score_gemma":0.023277042,"teacher_disagreement_score":0.01086751,"about_ca_system_score_codex":0.0002984153,"about_ca_system_score_gemma":0.00044612162,"threshold_uncertainty_score":0.021608472},"labels":[],"label_agreement":null},{"id":"W2072324595","doi":"10.1088/0004-637x/744/1/28","title":"A DIRECT MEASUREMENT OF THE TOTAL GAS COLUMN DENSITY IN ORION KL","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Eidgenössische Technische Hochschule Zürich; California Institute of Technology; National Aeronautics and Space Administration; Stockholms Universitet; Chalmers Tekniska Högskola; National Science Foundation","keywords":"Physics; Outflow; Ridge; Astrophysics; Plateau (mathematics); Line (geometry); Population; Radiation; Column (typography); Ultraviolet; Geometry; Nuclear physics; Optics; Meteorology","score_opus":0.022631427131162368,"score_gpt":0.21345684461907277,"score_spread":0.1908254174879104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072324595","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986223,0.000034739733,0.00042239885,0.000007990649,7.913919e-7,0.0000023319005,0.00023037288,0.000029820585,0.0006492614],"genre_scores_gemma":[0.9987515,0.000028639439,0.0006953181,0.000010020423,0.0000022375223,0.000005683768,0.0002873452,0.0000094299385,0.00020973664],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998989,0.000005262344,0.000004050895,0.000051777333,0.000021962616,0.000018034989],"domain_scores_gemma":[0.9997838,0.00003770394,0.00006924255,0.000024888812,0.000040198418,0.0000441593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013829047,0.0002621643,0.00022805962,0.00057193,0.00029931372,0.0004218352,0.00040913784,0.0001856248,0.0010922784],"category_scores_gemma":[0.00033565323,0.00020380905,0.00016855854,0.00042925184,0.0003082878,0.00052597874,0.00041340652,0.00025234115,0.00017513416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020327822,0.000075248674,0.6179891,0.00007232351,0.00009881408,0.0002569494,0.0006411937,0.002136981,0.36601478,0.00031422943,0.00017743367,0.0120195635],"study_design_scores_gemma":[0.000008598058,0.00008725029,0.9681521,0.000008498293,0.000039572762,0.00018972819,0.00022626946,0.004707391,0.025563832,0.00015814378,0.00084059924,0.000017967413],"about_ca_topic_score_codex":0.006118404,"about_ca_topic_score_gemma":0.007457956,"teacher_disagreement_score":0.006118404,"about_ca_system_score_codex":0.00032523795,"about_ca_system_score_gemma":0.0001495284,"threshold_uncertainty_score":0.012165606},"labels":[],"label_agreement":null},{"id":"W2072330130","doi":"10.1088/0004-637x/746/1/75","title":"STAR FORMATION IN MASSIVE CLUSTERS VIA BONDI ACCRETION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Star formation; Stars; Accretion (finance); Molecular cloud; Milky Way; Initial mass function; Star cluster; Mass distribution","score_opus":0.010371319508378597,"score_gpt":0.23879969028388354,"score_spread":0.22842837077550493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072330130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94255316,0.0007976889,0.023332981,0.00050662865,0.00009660964,0.000063459134,0.00009555862,0.00039305002,0.03216087],"genre_scores_gemma":[0.99472153,0.00031744046,0.0017712332,0.00003352109,0.000038016442,0.000027004424,0.00005691242,0.000038923838,0.0029953397],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986243,0.00002846299,0.000004214457,0.000036243633,0.000032899305,0.000035822068],"domain_scores_gemma":[0.99971455,0.00004465289,0.00009276123,0.000034666635,0.000017679122,0.000095691175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026257482,0.0005164465,0.00038072,0.0002960124,0.0011041531,0.0011348012,0.0008489778,0.00043816713,0.0015445873],"category_scores_gemma":[0.0012097002,0.00032831967,0.0003887057,0.0002495835,0.00089046307,0.0006478559,0.0016550906,0.00052713964,0.00064553635],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046284456,0.00019797249,0.072382204,0.00025616834,0.0002153426,0.0017546125,0.0010213938,0.36656797,0.029829657,0.49632052,0.008850198,0.02214113],"study_design_scores_gemma":[0.00010931825,0.00020612494,0.0255419,0.00003733418,0.000052391577,0.0005152817,0.00018506213,0.89744735,0.0034192824,0.067333244,0.005083255,0.00006947975],"about_ca_topic_score_codex":0.006885607,"about_ca_topic_score_gemma":0.003944948,"teacher_disagreement_score":0.006885607,"about_ca_system_score_codex":0.0014642515,"about_ca_system_score_gemma":0.0005160966,"threshold_uncertainty_score":0.013691068},"labels":[],"label_agreement":null},{"id":"W2072345977","doi":"10.1088/0004-637x/763/2/120","title":"THE ANATOMY OF AN EXTREME STARBURST WITHIN 1.3 Gyr OF THE BIG BANG REVEALED BY ALMA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Quasar; Galaxy; Astronomy; Submillimeter Array; Star formation; Redshift; Active galactic nucleus; Emission spectrum; Millimeter; Local Group; Spectral line; Milky Way","score_opus":0.008327755308544564,"score_gpt":0.20926466465657279,"score_spread":0.20093690934802821,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072345977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971163,0.0002668869,0.00023627061,0.00009331784,0.0000048807833,0.000003581372,0.00016969928,0.00002378206,0.002085267],"genre_scores_gemma":[0.9992009,0.00009699595,0.00017080612,0.000030376144,0.000007816447,0.000002021841,0.000090674825,0.0000041715593,0.0003962335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999948,0.000007173546,0.000002362135,0.000016355116,0.000006760944,0.000019225068],"domain_scores_gemma":[0.9997309,0.000036528596,0.00010682925,0.000027544242,0.000021394864,0.0000767474],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011234696,0.00013201051,0.00010983603,0.0008983266,0.0003155512,0.00047193604,0.00020183554,0.00025693735,0.0013510855],"category_scores_gemma":[0.00034976157,0.00014392544,0.00014221214,0.0003373615,0.00026985916,0.00027926525,0.00037293142,0.0003895619,0.00021409648],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046927846,0.00005664443,0.910184,0.000027363829,0.000042180516,0.004517518,0.0016016967,0.00017246477,0.0682636,0.0007253069,0.00041654028,0.013523381],"study_design_scores_gemma":[0.0000018280897,0.000045244815,0.99758184,0.000004714793,0.0000064698643,0.0010438457,0.00018963587,0.00010604194,0.0004522745,0.00012517443,0.0004392471,0.0000035076346],"about_ca_topic_score_codex":0.0049624667,"about_ca_topic_score_gemma":0.0075313137,"teacher_disagreement_score":0.0049624667,"about_ca_system_score_codex":0.0002198863,"about_ca_system_score_gemma":0.000098754346,"threshold_uncertainty_score":0.009867191},"labels":[],"label_agreement":null},{"id":"W2072390915","doi":"10.1086/503795","title":"Giant Planet Accretion and Migration: Surviving the Type I Regime","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gas giant; Physics; Planet; Accretion (finance); Giant planet; Astrophysics; Jovian; Astronomy; Planetary migration; Gravitational collapse; Protoplanetary disk; Astrobiology; Exoplanet; Planetary system","score_opus":0.00830409622852919,"score_gpt":0.2155819147935505,"score_spread":0.2072778185650213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072390915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.950033,0.002591194,0.016749196,0.0035097958,0.00014201217,0.000031217038,0.00024626963,0.0001847631,0.0265125],"genre_scores_gemma":[0.99640346,0.0006113121,0.00088178203,0.00018871589,0.0000700407,0.000011044898,0.000053314197,0.000014096144,0.0017662866],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998659,0.000026878779,0.0000060169386,0.00003324303,0.000015644631,0.000052440628],"domain_scores_gemma":[0.9990569,0.00021914166,0.00038351465,0.00012123915,0.000044407174,0.00017479196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046807277,0.00039696816,0.0004928927,0.00021989424,0.0010328566,0.001134678,0.00062026654,0.0014541218,0.001984995],"category_scores_gemma":[0.003219819,0.00020861458,0.0004962632,0.00022681076,0.0015119597,0.0024194298,0.0014273654,0.0007896895,0.0003672547],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087400444,0.00021898907,0.20014544,0.0004996117,0.00014743961,0.005516782,0.0022130045,0.08620166,0.022955874,0.609895,0.0076101497,0.06372201],"study_design_scores_gemma":[0.00022141398,0.0005973954,0.059151966,0.00017478512,0.00009397458,0.004914899,0.0012415231,0.19539557,0.00439634,0.7153582,0.018344948,0.000108990374],"about_ca_topic_score_codex":0.0029704731,"about_ca_topic_score_gemma":0.0012227707,"teacher_disagreement_score":0.0029704731,"about_ca_system_score_codex":0.000790694,"about_ca_system_score_gemma":0.00038915212,"threshold_uncertainty_score":0.0066404343},"labels":[],"label_agreement":null},{"id":"W2072444994","doi":"10.1088/0004-637x/706/1/319","title":"ON THE NATURE OF THE FIRST GALAXIES SELECTED AT 350 μm","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Luminous infrared galaxy; Redshift; Flux (metallurgy); Radio galaxy; Extinction (optical mineralogy); Star formation; Galaxy formation and evolution; Spectral energy distribution","score_opus":0.0037767735692477602,"score_gpt":0.18996570594873424,"score_spread":0.18618893237948647,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072444994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99043673,0.00040218787,0.00018172893,0.00022659861,0.000011148341,0.000009889918,0.001223967,0.000027549526,0.00748013],"genre_scores_gemma":[0.9981768,0.00006134136,0.00016734735,0.00004533989,0.000007802696,0.0000040034774,0.0006020625,0.000004265896,0.00093101757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982256,0.000017722223,0.0000061660007,0.00005312762,0.000037997503,0.00006243954],"domain_scores_gemma":[0.9980045,0.0005107713,0.00047589152,0.0001547515,0.00036618765,0.00048791766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035219744,0.00008209528,0.00009419151,0.0021905631,0.00069700443,0.0007220288,0.000312095,0.0003839427,0.0035260897],"category_scores_gemma":[0.0017492606,0.00011133117,0.000111302084,0.0009976341,0.00038744378,0.00044854835,0.00054245733,0.000312914,0.0006868113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022038212,0.000048278787,0.9712804,0.000019801297,0.000020730396,0.00023249813,0.0008373414,0.00010364012,0.0070728953,0.0011873592,0.0025481686,0.016428342],"study_design_scores_gemma":[0.0000014974573,0.0000067175606,0.99804246,0.0000042010133,0.0000029463538,0.00010674601,0.00029990007,0.000082066654,0.00022165394,0.00006745078,0.0011622935,0.0000020980428],"about_ca_topic_score_codex":0.017831802,"about_ca_topic_score_gemma":0.044269584,"teacher_disagreement_score":0.017831802,"about_ca_system_score_codex":0.00051037053,"about_ca_system_score_gemma":0.00022702776,"threshold_uncertainty_score":0.035456},"labels":[],"label_agreement":null},{"id":"W2072476494","doi":"10.1086/497026","title":"Far‐Ultraviolet and Optical Observations of BW Vulpeculae","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Light curve; Photometry (optics); Ultraviolet; Effective temperature; Spectral line; Amplitude; Line (geometry); Stellar atmosphere; Astronomy; Spectral energy distribution; Stars; Optics","score_opus":0.01637449571703301,"score_gpt":0.23170975670507873,"score_spread":0.21533526098804573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072476494","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982497,0.00005302548,0.00018671912,0.0000069426587,0.0000012500986,0.0000018128356,0.00021872543,0.000016040467,0.0012657328],"genre_scores_gemma":[0.99828786,0.00006517856,0.00039380003,0.000009775865,0.0000044201533,0.0000034364427,0.0008718886,0.000014403467,0.0003491345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989593,0.000008436157,0.0000030487286,0.000032179458,0.000031580475,0.000028698461],"domain_scores_gemma":[0.99987984,0.000014512846,0.000034442757,0.000016828648,0.000012993286,0.00004134325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013336621,0.00019873884,0.00014482233,0.0007182152,0.00036062632,0.0003115153,0.00022565934,0.00017814404,0.00058706995],"category_scores_gemma":[0.00030033704,0.00014817873,0.00015728307,0.0002933183,0.0002166401,0.00026347963,0.0004584442,0.00023174298,0.00020500377],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032915355,0.0001474886,0.72957873,0.00006870569,0.00014371934,0.0003342088,0.0009271063,0.0040859124,0.22436744,0.0011122873,0.0005113697,0.03839392],"study_design_scores_gemma":[0.000005992911,0.000067130764,0.9903439,0.000008936823,0.000015985333,0.00013961797,0.00012278123,0.0013033182,0.0059253997,0.00019230289,0.0018678345,0.00000683933],"about_ca_topic_score_codex":0.0038093731,"about_ca_topic_score_gemma":0.005756905,"teacher_disagreement_score":0.0038093731,"about_ca_system_score_codex":0.00028383275,"about_ca_system_score_gemma":0.0000944709,"threshold_uncertainty_score":0.0075743794},"labels":[],"label_agreement":null},{"id":"W2072477664","doi":"10.1088/0004-637x/712/2/1345","title":"NEW INSIGHTS INTO THE PROBLEM OF THE SURFACE GRAVITY DISTRIBUTION OF COOL DA WHITE DWARFS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Surface gravity; Spectral line; Helium; Mixing (physics); Convection; Effective temperature; Distribution (mathematics)","score_opus":0.00669633735224793,"score_gpt":0.21358134551441513,"score_spread":0.2068850081621672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072477664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9160623,0.004197858,0.06950632,0.0035319128,0.000045865327,0.000007651894,0.00046267023,0.00023770385,0.0059477817],"genre_scores_gemma":[0.99461347,0.0006920253,0.0037132984,0.00015382469,0.00013824069,0.000002652795,0.00018107909,0.00004975967,0.00045565606],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997527,0.000055582343,0.000013633839,0.000103533064,0.00004759767,0.000026994385],"domain_scores_gemma":[0.99875534,0.00048206243,0.00029415745,0.0002233638,0.00013430047,0.00011073783],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00075434387,0.0002847527,0.0006120384,0.0012022268,0.00045696797,0.0011619343,0.0008319094,0.000495378,0.00094696693],"category_scores_gemma":[0.0036885678,0.00017638621,0.00021610061,0.0012923325,0.001540465,0.0019867413,0.0010252348,0.0007609421,0.00017578797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002034485,0.0000553324,0.69880843,0.00017741168,0.00016864175,0.0007111515,0.0036052037,0.029486883,0.016848441,0.15693754,0.0037640352,0.08923354],"study_design_scores_gemma":[0.000032487216,0.00006577611,0.56096286,0.000043367272,0.000032912387,0.0015840385,0.0017642456,0.07098103,0.0022362212,0.34696406,0.015259278,0.00007379499],"about_ca_topic_score_codex":0.005239888,"about_ca_topic_score_gemma":0.0033156625,"teacher_disagreement_score":0.005239888,"about_ca_system_score_codex":0.0006032208,"about_ca_system_score_gemma":0.00015710604,"threshold_uncertainty_score":0.010418773},"labels":[],"label_agreement":null},{"id":"W2072494951","doi":"10.1086/424902","title":"Tidal Torques and the Orientation of Nearby Disk Galaxies","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Principal axis theorem; Rotation (mathematics); Angular momentum; Perpendicular; Orientation (vector space); Galaxy; Thick disk; Plane (geometry); Thin disk; Moment of inertia","score_opus":0.004718532635996359,"score_gpt":0.2083893918491782,"score_spread":0.20367085921318184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072494951","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950335,0.00009019535,0.00108242,0.000111880574,0.000012636695,0.000011565699,0.00017015393,0.00005595632,0.003431559],"genre_scores_gemma":[0.99896765,0.000033833636,0.00057487487,0.000014832516,0.0000026785074,0.0000069073653,0.000116593146,0.000013803727,0.00026887294],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989355,0.00002731211,0.0000060026623,0.000018572791,0.00002142826,0.00003310437],"domain_scores_gemma":[0.99885595,0.00048435119,0.00021846121,0.000095987685,0.000129483,0.00021576868],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000437869,0.00031881128,0.0003879518,0.00078513636,0.0007274259,0.0010859257,0.0007422316,0.00094921526,0.0015689468],"category_scores_gemma":[0.0036361888,0.00035133224,0.00039736816,0.0006987559,0.00090995076,0.00068268925,0.0006461069,0.00056468975,0.00022417215],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013931112,0.00013338774,0.04030001,0.000028007547,0.000054149772,0.00017229929,0.0001501983,0.9527813,0.001545642,0.0025612777,0.00037849136,0.0017559367],"study_design_scores_gemma":[0.000050419363,0.00004343856,0.007819949,0.000009920553,0.000016349037,0.000025360792,0.00012560711,0.99006265,0.00040242204,0.0010574276,0.0003721726,0.000014327113],"about_ca_topic_score_codex":0.036080383,"about_ca_topic_score_gemma":0.0197918,"teacher_disagreement_score":0.036080383,"about_ca_system_score_codex":0.0015185354,"about_ca_system_score_gemma":0.00067472237,"threshold_uncertainty_score":0.07174075},"labels":[],"label_agreement":null},{"id":"W2072575586","doi":"10.1086/430497","title":"Cepheid Calibrations from the<i>Hubble Space Telescope</i>of the Luminosity of Two Recent Type Ia Supernovae and a Redetermination of the Hubble Constant","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":194,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Hubble's law; Hubble space telescope; Physics; Supernova; Hubble Ultra-Deep Field; Astrophysics; Luminosity; Astronomy; Hubble Deep Field; Type (biology); Constant (computer programming); Cosmology; Stars; Galaxy; Computer science; Geology; Dark energy","score_opus":0.01155442642049818,"score_gpt":0.2396443605026012,"score_spread":0.22808993408210304,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072575586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7710804,0.0025789703,0.05661977,0.0016622241,0.0013852501,0.00014643196,0.062401418,0.003298947,0.10082671],"genre_scores_gemma":[0.9490545,0.00043631232,0.014023807,0.00015616803,0.00013634384,0.000057100715,0.02836174,0.00058360095,0.007190511],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99938774,0.000072130795,0.000032412798,0.0001782636,0.0002489394,0.0000804737],"domain_scores_gemma":[0.9950303,0.0011244817,0.0007919896,0.00096710515,0.0018522585,0.00023388394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001229253,0.00039877094,0.00024994023,0.001949701,0.0007145559,0.0007654517,0.00072495773,0.00067062816,0.0078233695],"category_scores_gemma":[0.006831146,0.00045455826,0.0002898907,0.001779422,0.00029762485,0.00060268835,0.0004793966,0.0009610673,0.0035435592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010127604,0.0001823733,0.58144224,0.0006875762,0.0003087808,0.00057122146,0.00092074176,0.044045836,0.03729914,0.03710594,0.12009679,0.17632657],"study_design_scores_gemma":[0.000075879376,0.000055403467,0.86242783,0.00006545055,0.00007537063,0.00030402097,0.00013712882,0.022466682,0.027327847,0.0061971773,0.080778785,0.00008842024],"about_ca_topic_score_codex":0.008066157,"about_ca_topic_score_gemma":0.019209614,"teacher_disagreement_score":0.008066157,"about_ca_system_score_codex":0.00080480805,"about_ca_system_score_gemma":0.00035262213,"threshold_uncertainty_score":0.026171803},"labels":[],"label_agreement":null},{"id":"W2072577922","doi":"10.1088/0004-637x/694/2/l148","title":"<i>HST</i> /NICMOS DETECTION OF HR 8799 b IN 1998","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; National Research Council Canada; Herzberg Institute of Astrophysics; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Exoplanet; Astrometry; Photometry (optics); Stars; Planetary system; James Webb Space Telescope; Spitzer Space Telescope","score_opus":0.007425973256244498,"score_gpt":0.21483609219093913,"score_spread":0.20741011893469463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072577922","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94982505,0.0005235638,0.0015679982,0.00029318506,0.00011371537,0.000046554094,0.02381339,0.00047636576,0.02334014],"genre_scores_gemma":[0.9399801,0.0005239063,0.010779241,0.0002996283,0.0001140058,0.00004583412,0.043344658,0.000082029124,0.004830607],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998723,0.0000063898724,0.00001101156,0.000030348301,0.000057849233,0.00002212599],"domain_scores_gemma":[0.99972004,0.000012840715,0.00010379027,0.000050598923,0.0000763487,0.000036311052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014756678,0.0001769718,0.00013371014,0.0018444001,0.00038176676,0.00042149576,0.00022802374,0.00020726678,0.0019308304],"category_scores_gemma":[0.00031181454,0.00008005838,0.00011711126,0.0011516929,0.00015284891,0.00015753401,0.00039910237,0.00022398883,0.0011188964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070699153,0.00021433466,0.658895,0.00029277027,0.00012034016,0.0024248175,0.0011405151,0.0009122276,0.16707706,0.00162425,0.048776485,0.11781521],"study_design_scores_gemma":[0.000009153738,0.000038392896,0.96192616,0.00003620084,0.00001893581,0.0010292974,0.00014664093,0.0006458537,0.012806437,0.00012369386,0.023210296,0.000008845714],"about_ca_topic_score_codex":0.009035347,"about_ca_topic_score_gemma":0.021856366,"teacher_disagreement_score":0.009035347,"about_ca_system_score_codex":0.0004058232,"about_ca_system_score_gemma":0.0002011518,"threshold_uncertainty_score":0.017965496},"labels":[],"label_agreement":null},{"id":"W2072610358","doi":"10.1086/345950","title":"Neutral Carbon in Post–Asymptotic Giant Branch Stars and Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canada Council for the Arts; University of Calgary","funders":"","keywords":"Planetary nebula; Asymptotic giant branch; Physics; Astrophysics; Stars; Carbon star; Astronomy; Carbon fibers; Atomic carbon; Line (geometry); Abundance (ecology); Nebula; Protoplanetary nebula; Hydrogen; Biology","score_opus":0.006012162691871115,"score_gpt":0.20235744968706393,"score_spread":0.19634528699519282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072610358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938774,0.0002642814,0.000014817061,0.0000066671246,6.900685e-7,7.3365476e-7,0.000023006372,7.1783614e-7,0.00030141958],"genre_scores_gemma":[0.9995468,0.00016490805,0.000033405635,0.0000074288323,0.0000033775386,0.0000010711682,0.00009373364,5.6859426e-7,0.00014876237],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995697,0.0000059751587,0.0000022249144,0.000009827124,0.000013734301,0.000011277312],"domain_scores_gemma":[0.9997795,0.00003468086,0.000076414064,0.000011078422,0.000037518228,0.000060782917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014435055,0.00012745292,0.00009519634,0.00076422794,0.00027735505,0.00027714384,0.00015355083,0.00025066166,0.0004419414],"category_scores_gemma":[0.0004032345,0.00009499684,0.00005892853,0.00038012597,0.000283668,0.0001710211,0.00021045763,0.00011475925,0.00008497506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026209193,0.000044441873,0.9737169,0.00001950887,0.000021103135,0.0005505633,0.00016154161,0.00009910664,0.019093027,0.00015505347,0.00006591042,0.0058106417],"study_design_scores_gemma":[0.0000033634437,0.000046904355,0.9979856,0.0000029592293,0.0000055692303,0.00070957764,0.000055466848,0.00006835564,0.0007353025,0.00010820319,0.00027765395,0.0000010595622],"about_ca_topic_score_codex":0.00488759,"about_ca_topic_score_gemma":0.0058134105,"teacher_disagreement_score":0.00488759,"about_ca_system_score_codex":0.00023640612,"about_ca_system_score_gemma":0.00010059047,"threshold_uncertainty_score":0.009718239},"labels":[],"label_agreement":null},{"id":"W2072676559","doi":"10.1088/0004-637x/785/1/42","title":"FRAGMENTATION OF MASSIVE DENSE CORES DOWN TO ≲ 1000 AU: RELATION BETWEEN FRAGMENTATION AND DENSITY STRUCTURE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria","funders":"","keywords":"Physics; Fragmentation (computing); Astrophysics; Density contrast; Power law; Turbulence; Computational physics; Mechanics; Statistics","score_opus":0.007128885802065719,"score_gpt":0.24048242569290218,"score_spread":0.23335353989083646,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072676559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99905854,0.00008692627,0.00039276943,0.000004008963,4.4276536e-7,0.000002958252,0.000042687792,0.000007841815,0.00040384592],"genre_scores_gemma":[0.9995759,0.000028689632,0.00023265868,0.0000021162307,0.0000011751155,0.0000014844215,0.00007850842,0.000001702849,0.000077792414],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999454,0.0000051974744,0.0000035254943,0.000013401682,0.000011705576,0.000020783635],"domain_scores_gemma":[0.99934405,0.00012599766,0.00027712045,0.00003606762,0.00010974577,0.00010708335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016411471,0.00012287864,0.0001383985,0.00073941547,0.0001993203,0.00031279112,0.00021004607,0.00014339038,0.0006249496],"category_scores_gemma":[0.0009953248,0.00015808159,0.00012449348,0.00034511977,0.00031508613,0.00022603682,0.00039274673,0.00013145129,0.00011974956],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005131193,0.00006742764,0.8870571,0.000055320295,0.00006444639,0.0007600932,0.00043064659,0.0075134397,0.09112398,0.00087833474,0.0001358065,0.011400318],"study_design_scores_gemma":[0.000007470742,0.00007338058,0.9821976,0.0000053632725,0.000009566303,0.00036428106,0.00008629475,0.010502847,0.006210835,0.00035445977,0.00018186377,0.0000060682682],"about_ca_topic_score_codex":0.003365485,"about_ca_topic_score_gemma":0.0021243254,"teacher_disagreement_score":0.003365485,"about_ca_system_score_codex":0.00029024607,"about_ca_system_score_gemma":0.000078061516,"threshold_uncertainty_score":0.0066918135},"labels":[],"label_agreement":null},{"id":"W2072795338","doi":"10.1088/0004-637x/787/2/164","title":"MODELING CONVECTIVE CORE OVERSHOOT AND DIFFUSION IN PROCYON CONSTRAINED BY ASTEROSEISMIC DATA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Convection; Adiabatic process; Diffusion; Core (optical fiber); RADIUS; Position (finance); Overshoot (microwave communication); Helium","score_opus":0.02091694257531883,"score_gpt":0.23918552022358622,"score_spread":0.21826857764826738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072795338","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99639195,0.00005716582,0.0028819703,0.000028174964,0.0000019162683,0.000004909133,0.0001166077,0.00004069374,0.0004766998],"genre_scores_gemma":[0.99807537,0.00003473985,0.0014793937,0.000006520214,0.000002026063,0.0000054834436,0.0001785154,0.000018724077,0.00019925623],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999052,0.000018985134,0.000004138657,0.00003800253,0.0000099669605,0.000023551927],"domain_scores_gemma":[0.9994598,0.00024120847,0.00012334196,0.00006188351,0.000038141545,0.00007566567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004378899,0.0004093766,0.00032636515,0.00040693817,0.0002681293,0.00061602,0.00073719985,0.0006611415,0.00072360283],"category_scores_gemma":[0.0015339223,0.0002884953,0.00042161628,0.00030182424,0.00039625584,0.00052534894,0.00060337776,0.00038691657,0.00012114051],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002447772,0.00004100426,0.097056836,0.000047956437,0.00006807144,0.00024545935,0.00020331836,0.89072627,0.004957564,0.0016935823,0.00017064184,0.0045444667],"study_design_scores_gemma":[0.000043223037,0.000060945942,0.025159957,0.000011213411,0.000022572784,0.000094615556,0.00007261583,0.9713118,0.0019687603,0.0008162351,0.0004220654,0.000016017391],"about_ca_topic_score_codex":0.013908832,"about_ca_topic_score_gemma":0.010148066,"teacher_disagreement_score":0.013908832,"about_ca_system_score_codex":0.0006973373,"about_ca_system_score_gemma":0.00040031844,"threshold_uncertainty_score":0.02765572},"labels":[],"label_agreement":null},{"id":"W2072891863","doi":"10.1086/591508","title":"Low‐Level Nuclear Activity in Nearby Spiral Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Hubble sequence; Supermassive black hole; Spiral galaxy; Dwarf galaxy; Barred spiral galaxy; Interacting galaxy; Spiral (railway)","score_opus":0.01519265729160881,"score_gpt":0.21449029323568,"score_spread":0.19929763594407118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2072891863","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995505,0.0000427474,0.000053924523,0.0000046864448,4.046023e-7,0.0000013093534,0.000027199047,0.000004353055,0.00031475906],"genre_scores_gemma":[0.99961805,0.000030817762,0.00013641283,0.000002734491,0.0000016872275,0.0000012988219,0.00007593162,8.843067e-7,0.00013217538],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998846,0.000015549369,0.0000093616145,0.00003130909,0.000028581784,0.000030548254],"domain_scores_gemma":[0.9994462,0.00007113433,0.00020602452,0.00006182416,0.00007295887,0.00014189733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020156131,0.00016411237,0.0001797402,0.0011803585,0.00031105414,0.0004613138,0.00020992653,0.0002146633,0.0013164587],"category_scores_gemma":[0.00062141946,0.00008959873,0.00012753461,0.0005373863,0.00041043578,0.00023029189,0.00036386782,0.00012059696,0.00026040955],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012699795,0.000019433206,0.9800307,0.000010882365,0.000009600595,0.00014027664,0.00016431935,0.0001031618,0.015807066,0.00008910303,0.000021576632,0.0034769627],"study_design_scores_gemma":[0.0000041646203,0.00010341835,0.99692935,0.0000045505158,0.00001085365,0.0004224105,0.00018081292,0.00025544027,0.0018170681,0.00010756802,0.000161449,0.0000029811013],"about_ca_topic_score_codex":0.002914755,"about_ca_topic_score_gemma":0.0043409597,"teacher_disagreement_score":0.002914755,"about_ca_system_score_codex":0.00023947466,"about_ca_system_score_gemma":0.00011180587,"threshold_uncertainty_score":0.0057955384},"labels":[],"label_agreement":null},{"id":"W2073021432","doi":"10.1088/0004-637x/762/1/48","title":"SPIRAL ARMS IN THE ASYMMETRICALLY ILLUMINATED DISK OF MWC 758 AND CONSTRAINTS ON GIANT PLANETS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":256,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Japan Society for the Promotion of Science; National Aeronautics and Space Administration; Ministry of Education, Culture, Sports, Science and Technology; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Exoplanet; Astrophysics; Planet; Debris disk; Astronomy; Brown dwarf; Planetary system; Accretion (finance); Spiral (railway); Spiral galaxy; Stars","score_opus":0.01271783002966659,"score_gpt":0.23996932521022138,"score_spread":0.2272514951805548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073021432","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99933076,0.000028578024,0.000035041714,0.000009843934,4.3751461e-7,0.0000015817458,0.000042974687,0.00000436979,0.0005464523],"genre_scores_gemma":[0.9996346,0.00001721818,0.00014624641,0.0000076306615,0.0000012525423,0.000002090608,0.00007563901,0.0000016485319,0.00011357456],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999498,0.0000028335023,0.0000032095484,0.000015203827,0.000010918131,0.00001796535],"domain_scores_gemma":[0.9998294,0.000025246081,0.00006854754,0.000012694394,0.000011701729,0.000052415315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006375,0.00019326624,0.000110493114,0.0009976627,0.00037981212,0.0004493443,0.00033908384,0.00027153388,0.0009945523],"category_scores_gemma":[0.00042360846,0.00013856516,0.000096442825,0.00045296783,0.0003488744,0.00019474422,0.00041217075,0.000101783364,0.00020519424],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031408307,0.00003479181,0.9026601,0.000035379795,0.000032542273,0.0013823458,0.0007403244,0.001001707,0.07879794,0.0006657517,0.00029925062,0.014035745],"study_design_scores_gemma":[0.000013431348,0.000033562726,0.994745,0.0000114718,0.00002064333,0.0005885358,0.0003247728,0.0011706894,0.0019015823,0.00020046125,0.0009828056,0.0000070162355],"about_ca_topic_score_codex":0.016474595,"about_ca_topic_score_gemma":0.045628995,"teacher_disagreement_score":0.016474595,"about_ca_system_score_codex":0.00057294726,"about_ca_system_score_gemma":0.00016120836,"threshold_uncertainty_score":0.0327574},"labels":[],"label_agreement":null},{"id":"W2073029559","doi":"10.1086/320060","title":"Great Circle Tidal Streams: Evidence for a Nearly Spherical Massive Dark Halo around the Milky Way","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":459,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Milky Way; Galactic halo; Galaxy; Galactic Center; Galactic tide; Galactic corona; Dwarf galaxy; Large Magellanic Cloud; Proper motion; Galactic plane","score_opus":0.03295364080768916,"score_gpt":0.3056084746832922,"score_spread":0.2726548338756031,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073029559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996909,0.000009504432,0.00013112144,0.0000049749838,4.494547e-7,0.0000025460404,0.000024787772,0.000010197583,0.00012555899],"genre_scores_gemma":[0.99958867,0.000009722326,0.00021193096,0.000004058221,0.0000011822764,0.0000019805182,0.00008548319,0.000003202391,0.00009376251],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999175,0.000022079394,0.0000055322166,0.000019414325,0.000019259789,0.000016198828],"domain_scores_gemma":[0.9990879,0.00031904803,0.00021824703,0.00012078878,0.00006013522,0.00019388889],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029677962,0.00016606966,0.00023756552,0.00034735524,0.0002823763,0.00034515664,0.0003479495,0.0002471895,0.0008104193],"category_scores_gemma":[0.0010671432,0.00017377663,0.0002367095,0.00022038246,0.00043400427,0.00018342149,0.00040791108,0.00013905848,0.00012926263],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011705839,0.00029346766,0.91611457,0.000045550943,0.00015183374,0.00078126194,0.0005898048,0.02515771,0.046934273,0.00089900615,0.00023722214,0.007624701],"study_design_scores_gemma":[0.0001111858,0.00084661203,0.8986585,0.000011091569,0.00008613925,0.00046051666,0.00035937145,0.088051625,0.010119138,0.0006132617,0.0006502985,0.0000322135],"about_ca_topic_score_codex":0.0045683663,"about_ca_topic_score_gemma":0.0065764715,"teacher_disagreement_score":0.0045683663,"about_ca_system_score_codex":0.00024027581,"about_ca_system_score_gemma":0.00015444538,"threshold_uncertainty_score":0.009083569},"labels":[],"label_agreement":null},{"id":"W2073236198","doi":"10.1086/379344","title":"The Mass Function of Supergiant Molecular Complexes and Implications for Forming Young Massive Star Clusters in the Antennae (NGC 4038/4039)","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Physics; Molecular cloud; Star formation; Galaxy; Spiral galaxy; Supergiant; Cluster (spacecraft); Astronomy; Star cluster; Stars","score_opus":0.008471196934405215,"score_gpt":0.21933992483358378,"score_spread":0.21086872789917857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073236198","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99874675,0.00008556332,0.00016008002,0.00003085972,0.0000010663985,0.00000199931,0.000061144216,0.000010508937,0.0009019912],"genre_scores_gemma":[0.9994209,0.000034266475,0.00018913762,0.000006963543,0.00000237129,0.0000024641176,0.00008120027,0.0000042826705,0.0002584184],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990606,0.0000092766295,0.0000043424443,0.000034875568,0.00001897552,0.000026554086],"domain_scores_gemma":[0.99947065,0.000075888354,0.0002468566,0.0000478089,0.00004598241,0.00011274952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002706151,0.00024983182,0.0002102811,0.0007465958,0.00026279222,0.00048432432,0.0003735235,0.00025678184,0.0009270404],"category_scores_gemma":[0.0009165058,0.0001962732,0.00019704725,0.0004963093,0.00030143198,0.000398256,0.00037846935,0.00021871159,0.0002768845],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011752294,0.000029933008,0.9322243,0.000025507763,0.000035594156,0.00047878997,0.0005212994,0.0032376365,0.055431206,0.0009918918,0.0002140286,0.0066922633],"study_design_scores_gemma":[0.000005130811,0.000031122894,0.9947036,0.0000028965567,0.0000053639683,0.00021079129,0.000092405295,0.0025099353,0.0016144459,0.0003095451,0.0005077258,0.000007040945],"about_ca_topic_score_codex":0.004905694,"about_ca_topic_score_gemma":0.004581439,"teacher_disagreement_score":0.004905694,"about_ca_system_score_codex":0.0006809274,"about_ca_system_score_gemma":0.00009651505,"threshold_uncertainty_score":0.0097543},"labels":[],"label_agreement":null},{"id":"W2073238851","doi":"10.1088/0004-637x/720/1/923","title":"GAS EMISSION FROM DEBRIS DISKS AROUND A AND F STARS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Photoelectric effect; Debris; Debris disk; Cosmic dust; Stars; Sublimation (psychology); Spectral line; Thermal; Emission spectrum","score_opus":0.008880993697435039,"score_gpt":0.23881599725300767,"score_spread":0.22993500355557264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073238851","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99876714,0.0000498194,0.00019726931,0.000010048045,0.0000013339104,0.0000030292,0.00014926301,0.000042638767,0.0007795102],"genre_scores_gemma":[0.99822634,0.000044140033,0.00086582644,0.000013582045,0.0000029181192,0.00000495322,0.0003978882,0.000017967943,0.00042619117],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996424,0.000002436655,0.0000016692002,0.000011690045,0.000010586154,0.000009308711],"domain_scores_gemma":[0.9998926,0.000024491503,0.000024076984,0.000009796521,0.000019606377,0.00002944563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000077035176,0.00013888911,0.00012637429,0.0003563537,0.00030154467,0.00021215888,0.00023621216,0.00016403882,0.00073971925],"category_scores_gemma":[0.00021052324,0.00010335214,0.00015310009,0.00022786226,0.00015644635,0.00010110149,0.00020333873,0.00013936365,0.00016406292],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005258039,0.00012917048,0.5352343,0.00010043521,0.000082594626,0.001041209,0.00072752597,0.011841837,0.42706445,0.00054295384,0.001122251,0.021587543],"study_design_scores_gemma":[0.00006383507,0.00016693404,0.95440465,0.000013527842,0.000026062371,0.00041448465,0.0001854286,0.01713821,0.024295606,0.00022544706,0.0030528521,0.000012938701],"about_ca_topic_score_codex":0.0060416805,"about_ca_topic_score_gemma":0.004099291,"teacher_disagreement_score":0.0060416805,"about_ca_system_score_codex":0.0004738853,"about_ca_system_score_gemma":0.00013493022,"threshold_uncertainty_score":0.012013018},"labels":[],"label_agreement":null},{"id":"W2073260115","doi":"10.1088/0004-637x/798/2/117","title":"ON THE DYNAMICS OF ULTRA COMPACT X-RAY BINARIES: 4U 1850-087, 4U 0513-40, AND M15 X-2","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; X-ray; Globular cluster; Dissipation; Quantum mechanics; Stars","score_opus":0.020921220961414407,"score_gpt":0.23909986646765047,"score_spread":0.21817864550623606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073260115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991579,0.00006338556,0.00015685757,0.00001536736,0.0000020405434,0.0000019486047,0.000032534437,0.000002848877,0.0005672492],"genre_scores_gemma":[0.9994849,0.00003531759,0.00016445183,0.0000063792445,0.0000018746647,0.0000019167087,0.00009375671,0.0000018663698,0.00020941818],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996305,0.0000053176273,0.0000020222258,0.000012578621,0.000006642839,0.00001038506],"domain_scores_gemma":[0.9999101,0.000011984845,0.000031411877,0.000006649193,0.000008603776,0.000031189247],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011473156,0.00015626595,0.00022811309,0.00039743716,0.00045373468,0.0003850745,0.0002531776,0.00016585698,0.00089320267],"category_scores_gemma":[0.00026817073,0.00008824416,0.00016821992,0.00035646054,0.0002828187,0.00030207526,0.0005947007,0.0001373731,0.00014318297],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040825413,0.00009242998,0.9279221,0.00006225182,0.00014237917,0.0008751075,0.000878975,0.029851869,0.018426757,0.0064531765,0.00053702644,0.014349565],"study_design_scores_gemma":[0.00002174155,0.00012270424,0.9239311,0.000016220636,0.000050099297,0.00024491784,0.0004983416,0.06901987,0.0019753608,0.0020552594,0.0020411117,0.000023228362],"about_ca_topic_score_codex":0.010378216,"about_ca_topic_score_gemma":0.010740607,"teacher_disagreement_score":0.010378216,"about_ca_system_score_codex":0.0006189661,"about_ca_system_score_gemma":0.00026626885,"threshold_uncertainty_score":0.020635605},"labels":[],"label_agreement":null},{"id":"W2073279969","doi":"10.1086/500380","title":"Evolutionary Synthesis Models of Young Star‐forming Regions: The Influence of Binary Stars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; McGill University","funders":"","keywords":"Physics; Astrophysics; Stars; Supernova; Stellar evolution; Interstellar medium; Roche lobe; Astronomy; Stellar mass loss; Binary star; Population; Star formation; Binary number; Galaxy","score_opus":0.010859183811202,"score_gpt":0.21983467133731005,"score_spread":0.20897548752610806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073279969","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8574192,0.0009472042,0.12780902,0.0001715251,0.000039780403,0.00008811842,0.0018355474,0.00058726483,0.011102336],"genre_scores_gemma":[0.981794,0.00046212043,0.013105318,0.000034647564,0.000025614967,0.00012228088,0.0008174576,0.00015031052,0.003488235],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998677,0.00004389658,0.0000072636153,0.000032742006,0.000022185219,0.000026239582],"domain_scores_gemma":[0.9991536,0.00043097534,0.00016935561,0.000059337937,0.0000871625,0.000099459954],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005584406,0.0005643193,0.00052806595,0.0006051303,0.00035264177,0.0009405458,0.0011514544,0.00060264353,0.0030152604],"category_scores_gemma":[0.0022196982,0.0003367789,0.0007503662,0.00037730666,0.00034701978,0.0006204427,0.0006527826,0.00030379946,0.0006239821],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007530805,0.000016713422,0.0059693744,0.000053932294,0.000035808847,0.00009670703,0.00008094243,0.97996145,0.0036498124,0.0052056843,0.00016833434,0.0046859407],"study_design_scores_gemma":[0.000026682736,0.000027222399,0.0018676843,0.0000057723737,0.000021539434,0.000038826704,0.000012752544,0.99379796,0.0007428721,0.0027988441,0.000652389,0.000007548307],"about_ca_topic_score_codex":0.008672894,"about_ca_topic_score_gemma":0.0034172258,"teacher_disagreement_score":0.008672894,"about_ca_system_score_codex":0.00089500996,"about_ca_system_score_gemma":0.0004137651,"threshold_uncertainty_score":0.017244816},"labels":[],"label_agreement":null},{"id":"W2073279988","doi":"10.1088/0004-637x/721/2/1900","title":"ROTATIONAL SPLITTING OF PULSATION MODES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Rotation (mathematics); Physics; Differential rotation; Mode (computer interface); Stars; Angular momentum; Astrophysics; Angular velocity; Classical mechanics; Geometry; Mathematics","score_opus":0.009818364766563052,"score_gpt":0.232502341070107,"score_spread":0.22268397630354395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073279988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99020153,0.00009304946,0.0065323757,0.00002020715,0.0000072397124,0.000010080546,0.00016816493,0.000095826355,0.0028716244],"genre_scores_gemma":[0.9986298,0.000024437582,0.0009546696,0.0000022339045,0.0000023259188,0.000007287991,0.00017185094,0.00001929823,0.00018804082],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99990535,0.000013557769,0.000007196523,0.00002700304,0.000023776729,0.000023154817],"domain_scores_gemma":[0.99954,0.000100551915,0.00010984719,0.000097901575,0.000089717956,0.000062043066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025934263,0.00037079095,0.00019932428,0.00069975184,0.00026799054,0.000450646,0.0002693772,0.00018236904,0.0014022272],"category_scores_gemma":[0.0015293552,0.00019893545,0.00039271114,0.00051850925,0.00034205953,0.00034326417,0.00039949006,0.0002562565,0.0001862089],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078246545,0.000090495145,0.13237767,0.00015186769,0.00012554221,0.00051654567,0.00023406018,0.7397899,0.07453401,0.018468242,0.0007969692,0.032132246],"study_design_scores_gemma":[0.000051447067,0.00020479936,0.06630883,0.0000113256965,0.000034849952,0.00034533092,0.00007460681,0.91709435,0.010111789,0.004985099,0.00074414065,0.000033498767],"about_ca_topic_score_codex":0.0010424937,"about_ca_topic_score_gemma":0.00055697444,"teacher_disagreement_score":0.0014022272,"about_ca_system_score_codex":0.0003492596,"about_ca_system_score_gemma":0.00016670539,"threshold_uncertainty_score":0.004690945},"labels":[],"label_agreement":null},{"id":"W2073335816","doi":"10.1086/323856","title":"Molecular Line Emissions from the Photodissociation Region of NGC 7027","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canada Council for the Arts; University of Calgary","funders":"","keywords":"Photodissociation; Planetary nebula; Physics; Line (geometry); Spectral line; Astrophysics; Emission spectrum; Atomic physics; Electron density; Molecule; Excitation; Electron; Chemistry; Photochemistry; Astronomy; Stars","score_opus":0.012599956604372433,"score_gpt":0.2456369625899305,"score_spread":0.23303700598555807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073335816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999323,0.00007695481,0.00009155795,0.0000055722708,6.426909e-7,0.0000016329022,0.00010025014,0.000010869069,0.00038951877],"genre_scores_gemma":[0.99839646,0.00018841705,0.0003054839,0.000013795071,0.0000022648978,0.000005951184,0.0005983734,0.0000072405983,0.0004820515],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99988365,0.000005740519,0.000003325014,0.000025099493,0.00003159319,0.000050512022],"domain_scores_gemma":[0.9998654,0.000017709366,0.00003974421,0.000013188425,0.000026406009,0.00003751476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000089268266,0.00036823808,0.00020250908,0.00073094975,0.00046294968,0.00040802755,0.00032940728,0.00021520143,0.0007297248],"category_scores_gemma":[0.00018913709,0.00019697643,0.00012422857,0.0006896556,0.00033695908,0.0001650102,0.00031181957,0.00018494514,0.0002247727],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036047344,0.00013406714,0.38739854,0.00012223529,0.00011246365,0.0012524894,0.0011247454,0.0019914203,0.59383225,0.0005933207,0.0007017357,0.012376286],"study_design_scores_gemma":[0.000027536684,0.00023502992,0.91589606,0.000014510356,0.000077965306,0.001166822,0.0004883427,0.0014468268,0.07507054,0.00018568404,0.005361053,0.000029674698],"about_ca_topic_score_codex":0.013797558,"about_ca_topic_score_gemma":0.01925368,"teacher_disagreement_score":0.013797558,"about_ca_system_score_codex":0.00070201687,"about_ca_system_score_gemma":0.00026932557,"threshold_uncertainty_score":0.027434468},"labels":[],"label_agreement":null},{"id":"W2073359418","doi":"10.1088/0004-637x/710/1/421","title":"EFFECTS OF α-ELEMENT ENHANCEMENT AND THE THERMALLY PULSING-ASYMPTOTIC GIANT BRANCH ON SURFACE BRIGHTNESS FLUCTUATION MAGNITUDES AND BROADBAND COLORS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Brightness; Red-giant branch; Stars; Surface brightness; Broadband; Giant star; Red giant","score_opus":0.0038609360669435216,"score_gpt":0.2058885386581963,"score_spread":0.2020276025912528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073359418","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99776673,0.00013654419,0.00065403996,0.000019921445,0.0000024526885,0.000002372059,0.00005441462,0.000017524737,0.0013459653],"genre_scores_gemma":[0.9995772,0.000046135396,0.00020891866,0.0000059843956,0.000002596454,0.0000013593676,0.00006204621,0.0000058949377,0.00008983543],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998872,0.000033568926,0.0000062932463,0.000034068013,0.000019703857,0.000019122308],"domain_scores_gemma":[0.9985922,0.00072207843,0.00039054532,0.00011060354,0.00009767209,0.000086859516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035749577,0.00029958406,0.0001545802,0.0003962024,0.000124531,0.0003664739,0.00019006849,0.00018790919,0.00085604173],"category_scores_gemma":[0.002110521,0.00015091611,0.00033233294,0.00024711597,0.00025168541,0.0002402497,0.00035052496,0.0001974486,0.0001424555],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005487749,0.000046667887,0.9114137,0.000058730908,0.0001452224,0.00038815208,0.00011293429,0.027724124,0.04114091,0.00094966445,0.00012649405,0.017344749],"study_design_scores_gemma":[0.000016333734,0.00022182263,0.96186393,0.000010212796,0.00010766108,0.00030116877,0.00004740868,0.02775089,0.008794852,0.0004708806,0.00040579887,0.000009062778],"about_ca_topic_score_codex":0.001559408,"about_ca_topic_score_gemma":0.0017056682,"teacher_disagreement_score":0.001559408,"about_ca_system_score_codex":0.00022541397,"about_ca_system_score_gemma":0.000090534544,"threshold_uncertainty_score":0.0031006932},"labels":[],"label_agreement":null},{"id":"W2073384938","doi":"10.1088/0004-637x/733/2/96","title":"GAMMA-RAY OBSERVATIONS OF THE Be/PULSAR BINARY 1A 0535+262 DURING A GIANT X-RAY OUTBURST","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Purdue University; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution; Science Foundation Ireland; National Science Foundation","keywords":"Physics; Pulsar; Astrophysics; Fermi Gamma-ray Space Telescope; Binary pulsar; X-ray; Population; Gamma ray; Black-body radiation; Astronomy; Photon; Luminosity; X-ray binary; High energy; Neutron star; Radiation; Millisecond pulsar; Nuclear physics; Galaxy","score_opus":0.026355442256162057,"score_gpt":0.215950401284948,"score_spread":0.18959495902878593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073384938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991454,0.000044507233,0.00003003287,0.0000074626228,0.0000012460285,0.0000031663108,0.00013888687,0.0000071425807,0.0006222075],"genre_scores_gemma":[0.99890935,0.000052762854,0.0002174836,0.000014158819,0.00000504354,0.0000032196292,0.00056458614,0.0000032749688,0.00023000987],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.0000048469306,0.000004954094,0.000015150956,0.000014918481,0.0000137976685],"domain_scores_gemma":[0.9998728,0.00000924555,0.00005093702,0.00001107691,0.00001469068,0.000041293784],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011304461,0.00020028217,0.00019412207,0.0007411407,0.0003513331,0.00029127923,0.00020962191,0.0002244059,0.000562363],"category_scores_gemma":[0.0001813031,0.000109800945,0.00013959,0.00054373906,0.00012534755,0.00013336989,0.00032247955,0.000255983,0.00014110129],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092112296,0.00027046367,0.8048147,0.00008249647,0.00010097419,0.001995663,0.00076825276,0.00084266334,0.17490235,0.00038492563,0.0007168614,0.014199395],"study_design_scores_gemma":[0.000007126967,0.00010486153,0.99689937,0.0000057611337,0.000016341397,0.00043339268,0.00009073867,0.00030424865,0.0015149014,0.000020469844,0.00059921405,0.0000035267283],"about_ca_topic_score_codex":0.004223971,"about_ca_topic_score_gemma":0.01226418,"teacher_disagreement_score":0.004223971,"about_ca_system_score_codex":0.00022772716,"about_ca_system_score_gemma":0.000109272325,"threshold_uncertainty_score":0.008398771},"labels":[],"label_agreement":null},{"id":"W2073451155","doi":"10.1086/508144","title":"Model Atmosphere Analysis of the Weakly Magnetic DZ White Dwarf G165‐7","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Zeeman effect; Spectral line; Polarization (electrochemistry); Sky; Magnetic field; Stellar atmosphere; Flux (metallurgy); Absorption spectroscopy","score_opus":0.007069264901443961,"score_gpt":0.20050269257940254,"score_spread":0.19343342767795857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073451155","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9620355,0.00022868316,0.008598291,0.00029730884,0.000077290795,0.000059752474,0.019754564,0.002053263,0.0068953573],"genre_scores_gemma":[0.9742606,0.00016259222,0.006868917,0.000076111595,0.000038920254,0.00007812844,0.016324313,0.00034708672,0.0018434296],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999201,0.000020320747,0.0000033823208,0.0000259799,0.000015944814,0.000014211721],"domain_scores_gemma":[0.999866,0.000028500412,0.000014247889,0.000022606311,0.000039608018,0.000029025694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019698883,0.00054878695,0.00047704828,0.0003449808,0.0004187296,0.0004912227,0.001019243,0.0003960659,0.00178646],"category_scores_gemma":[0.00044782294,0.0002405417,0.00059382414,0.0004639423,0.00015071881,0.00026710032,0.00027742432,0.00040491085,0.00057411246],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031434363,0.00017586963,0.069976196,0.00010239931,0.00037475547,0.00032649713,0.00021122275,0.8888857,0.013204685,0.0035090717,0.0104254875,0.012493822],"study_design_scores_gemma":[0.00028879519,0.00006523768,0.053337954,0.000005349874,0.00009332611,0.00007119953,0.0000645881,0.93458396,0.001911893,0.0009190325,0.008617931,0.000040677987],"about_ca_topic_score_codex":0.07887746,"about_ca_topic_score_gemma":0.04045368,"teacher_disagreement_score":0.07887746,"about_ca_system_score_codex":0.0010188965,"about_ca_system_score_gemma":0.0007046433,"threshold_uncertainty_score":0.15683669},"labels":[],"label_agreement":null},{"id":"W2073476240","doi":"10.1088/0004-637x/787/2/147","title":"THE COS/UVES ABSORPTION SURVEY OF THE MAGELLANIC STREAM. III. IONIZATION, TOTAL MASS, AND INFLOW RATE ONTO THE MILKY WAY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Toronto","funders":"","keywords":"Milky Way; Galaxy; Halo; Large Magellanic Cloud; Photoionization; Ionization; Small Magellanic Cloud","score_opus":0.007294204271203426,"score_gpt":0.2104370721555973,"score_spread":0.20314286788439387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073476240","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9876852,0.00067867705,0.00021552172,0.000081643826,0.00000984812,0.000010563767,0.0046624383,0.000059206275,0.006596962],"genre_scores_gemma":[0.9906893,0.00043958606,0.0005770331,0.00003832597,0.00002252612,0.000007696735,0.0056932336,0.000017732966,0.0025145612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999211,0.000008000713,0.0000041323415,0.000014245005,0.000025952613,0.000026493344],"domain_scores_gemma":[0.9997311,0.000010858741,0.00008997299,0.00001638044,0.00008147583,0.000070180315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013428114,0.00018084573,0.00010483389,0.002245701,0.0003172011,0.0003243205,0.00015020563,0.00011410248,0.0017129586],"category_scores_gemma":[0.00028012175,0.00007648852,0.00018641425,0.0010484179,0.000081722705,0.00017785144,0.00023815039,0.00013549378,0.0005060399],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006228759,0.000025981308,0.9736607,0.00002733438,0.000040223524,0.0000748766,0.00014682456,0.00016380106,0.008153091,0.00020469235,0.0027479955,0.014692312],"study_design_scores_gemma":[0.0000011252923,0.0000051706024,0.9979158,0.000003134487,0.0000032806565,0.00001629034,0.00003323197,0.00009369491,0.00033184292,0.000010102686,0.0015857769,6.0417636e-7],"about_ca_topic_score_codex":0.057854243,"about_ca_topic_score_gemma":0.089331016,"teacher_disagreement_score":0.057854243,"about_ca_system_score_codex":0.0005838775,"about_ca_system_score_gemma":0.00025974103,"threshold_uncertainty_score":0.115035},"labels":[],"label_agreement":null},{"id":"W2073564764","doi":"10.1086/383610","title":"H<scp>i</scp>Absorption of Polarized Emission: A New Technique for Determining Kinematic Distances to Galactic Supernova Remnants","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Supernova; Nebula; Absorption (acoustics); Polarization (electrochemistry); Pulsar; Supernova remnant; Astronomy; Stars; Optics","score_opus":0.01395155534716627,"score_gpt":0.2553955909053059,"score_spread":0.24144403555813962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073564764","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88379794,0.0014241957,0.105309814,0.00013575424,0.00004044014,0.000022310238,0.0005461096,0.0008671496,0.007856227],"genre_scores_gemma":[0.9526015,0.0005287954,0.045455225,0.000046344463,0.00004334247,0.00002512427,0.00031279458,0.00007816732,0.0009087527],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.99993455,0.000009702327,0.0000024887188,0.000020997453,0.000021656468,0.000010501006],"domain_scores_gemma":[0.9997534,0.00004160261,0.0000970545,0.000040025665,0.000044795637,0.000023109584],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011425817,0.00018702225,0.00009561538,0.00088222045,0.00017563769,0.00032158673,0.00032986046,0.00021486172,0.0006220242],"category_scores_gemma":[0.00027277548,0.00013914907,0.00012530835,0.00042705116,0.00026893988,0.0003963114,0.00024025475,0.00040493908,0.00024475917],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024626742,0.00004993207,0.097218916,0.00010318004,0.00008383455,0.00032059988,0.0001597328,0.0019764004,0.81493497,0.0019140708,0.0007152674,0.08227676],"study_design_scores_gemma":[0.000054406726,0.00044230037,0.30741695,0.000034571312,0.000117122894,0.0026477135,0.0001651934,0.044136707,0.6306256,0.0031425082,0.011119769,0.00009718195],"about_ca_topic_score_codex":0.0009518638,"about_ca_topic_score_gemma":0.0014229598,"teacher_disagreement_score":0.0009518638,"about_ca_system_score_codex":0.00012189601,"about_ca_system_score_gemma":0.000083538485,"threshold_uncertainty_score":0.0020809174},"labels":[],"label_agreement":null},{"id":"W2073673032","doi":"10.1086/444611","title":"The Structure of Close Binaries in Two Dimensions","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Roche lobe; Astrophysics; Stellar evolution; Stars; Binary number; Binary star; Equipotential; Stellar structure; Stellar mass; Star (game theory); Rotation (mathematics); Mass transfer; Star formation; Geometry; Thermodynamics","score_opus":0.006684741443938879,"score_gpt":0.23945600674506226,"score_spread":0.23277126530112338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073673032","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9893405,0.00021019712,0.00687542,0.00004081807,0.000009688912,0.000014503157,0.00011304343,0.00006264787,0.0033332189],"genre_scores_gemma":[0.9953584,0.000081207705,0.0034061933,0.000015820659,0.000007755402,0.000010779105,0.00023228498,0.000028706721,0.0008588208],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998567,0.000031844647,0.000007646119,0.000035954283,0.000034756315,0.000033004486],"domain_scores_gemma":[0.9995493,0.000109101005,0.000096333286,0.000051458122,0.0000661425,0.00012768892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002249783,0.000369528,0.0007127112,0.001056496,0.0009634317,0.0015899129,0.0006906764,0.000874984,0.003074351],"category_scores_gemma":[0.0012948774,0.000591518,0.0004962372,0.0006628557,0.0005997856,0.0012435048,0.001480838,0.0005927407,0.00028938233],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040395922,0.0002855303,0.06579329,0.0001322636,0.00016955179,0.0012926577,0.0006284252,0.86966395,0.010105142,0.038124114,0.0008266798,0.012574445],"study_design_scores_gemma":[0.000055977787,0.00012039171,0.019564748,0.0000117449335,0.000024191444,0.00027441833,0.00014289345,0.9638441,0.0013642376,0.013241137,0.0013244522,0.00003176759],"about_ca_topic_score_codex":0.005042703,"about_ca_topic_score_gemma":0.0031532086,"teacher_disagreement_score":0.005042703,"about_ca_system_score_codex":0.0007892445,"about_ca_system_score_gemma":0.00029018326,"threshold_uncertainty_score":0.010284722},"labels":[],"label_agreement":null},{"id":"W2073715627","doi":"10.1088/0004-637x/743/1/39","title":"STAR FORMATION AND YOUNG STELLAR CONTENT IN THE W3 GIANT MOLECULAR CLOUD","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Star formation; Astrophysics; Physics; Stars; Molecular cloud; Protostar; Young stellar object; Population; Astronomy; Star (game theory)","score_opus":0.025362666380769183,"score_gpt":0.22162557283370524,"score_spread":0.19626290645293606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073715627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997099,0.000031224128,0.00005567327,0.0000040830555,2.5670136e-7,0.0000010890094,0.000064983455,0.0000023687544,0.00013049184],"genre_scores_gemma":[0.9995654,0.000024062909,0.0001223165,0.0000043100513,0.000001257131,0.0000011426371,0.00020416794,0.0000029335317,0.00007430398],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999559,0.0000031295124,0.0000027896751,0.000011247709,0.000009302554,0.000017684199],"domain_scores_gemma":[0.9998012,0.000016850641,0.0000928367,0.000015884183,0.000025201613,0.00004803113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009897815,0.00010049843,0.00013805398,0.0006303465,0.0003088668,0.00039162437,0.0001376524,0.00014575094,0.00062561047],"category_scores_gemma":[0.00022551006,0.0000620043,0.00015321984,0.0006303855,0.00021082697,0.00025620178,0.00037563962,0.00013390317,0.00017828676],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009988818,0.000018715937,0.9665214,0.000013236915,0.0000231448,0.00015199206,0.00024939116,0.00025140855,0.028780393,0.0001416457,0.000048554986,0.003700231],"study_design_scores_gemma":[0.000001117069,0.000017922039,0.9983966,0.000001981865,0.0000040398554,0.000107830456,0.00011178705,0.00033314904,0.00080508133,0.00005661306,0.00016238911,0.0000015510801],"about_ca_topic_score_codex":0.005530175,"about_ca_topic_score_gemma":0.008247319,"teacher_disagreement_score":0.005530175,"about_ca_system_score_codex":0.00024843964,"about_ca_system_score_gemma":0.00015550922,"threshold_uncertainty_score":0.010995984},"labels":[],"label_agreement":null},{"id":"W2073845444","doi":"10.1086/508679","title":"The Global Evolution of Giant Molecular Clouds. I. Model Formulation and Quasi‐Equilibrium Behavior","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":198,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Galaxy; Star formation; Virial theorem; Photoevaporation; Stars; Astronomy","score_opus":0.0063310748108881005,"score_gpt":0.23258756661838376,"score_spread":0.22625649180749566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073845444","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47964153,0.0022428948,0.40132812,0.0037336226,0.00019830065,0.00021944825,0.0022241387,0.0007860899,0.109625824],"genre_scores_gemma":[0.9719463,0.0008309512,0.014895075,0.00019651534,0.00007128774,0.00028001113,0.00046404786,0.00014211712,0.011173747],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999324,0.000024320607,0.000002847398,0.000013214187,0.000013203832,0.0000140056045],"domain_scores_gemma":[0.99983966,0.000049226706,0.00004224468,0.000014283158,0.000026570027,0.000027995004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020583345,0.00061529095,0.00034247118,0.0003018156,0.000573363,0.0010310443,0.0012889133,0.0010547624,0.0025566842],"category_scores_gemma":[0.0008148895,0.00035932023,0.000681933,0.0003234729,0.0009295386,0.001339963,0.0009094662,0.0006112022,0.00049584854],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024586412,0.000020404072,0.001510971,0.000039418195,0.000021078644,0.00015391692,0.000113140224,0.89107317,0.0013907774,0.10295318,0.0009804104,0.0017189131],"study_design_scores_gemma":[0.000011468996,0.00001336916,0.0002836549,0.000006450437,0.0000052828495,0.000027489166,0.000025342953,0.9846467,0.0000708445,0.013562248,0.0013413725,0.000005845295],"about_ca_topic_score_codex":0.012563599,"about_ca_topic_score_gemma":0.0050906665,"teacher_disagreement_score":0.012563599,"about_ca_system_score_codex":0.0015171444,"about_ca_system_score_gemma":0.00067770074,"threshold_uncertainty_score":0.024980903},"labels":[],"label_agreement":null},{"id":"W2073900001","doi":"10.1086/524135","title":"The Detection of Molecular Gas in the Outskirts of NGC 6946","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Metallicity; Molecular cloud; Line (geometry); Star formation; Free molecular flow; Emission spectrum","score_opus":0.006051358832882363,"score_gpt":0.23373573876616519,"score_spread":0.22768437993328283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073900001","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904305,0.00009737905,0.00010002287,0.000007361146,0.000002142518,0.0000021646188,0.00013196096,0.000013896703,0.00060203613],"genre_scores_gemma":[0.9990152,0.00014945064,0.00022066383,0.000012321814,0.0000067053265,0.0000022678212,0.00027343488,0.000004565376,0.00031537452],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998374,0.000020364983,0.000009960602,0.00003881808,0.00004064881,0.000052768173],"domain_scores_gemma":[0.9996001,0.00003867342,0.0001405581,0.00003725168,0.000041603133,0.0001417451],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010557938,0.00028661787,0.0002681945,0.0008534006,0.0006573494,0.0005465486,0.00021182961,0.0002749468,0.0010363064],"category_scores_gemma":[0.00035207949,0.00014757874,0.00019026431,0.00043171216,0.00024737648,0.00021831076,0.00038920445,0.00016174663,0.00032292563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004166686,0.00008854109,0.682456,0.00006519745,0.000054609645,0.0014552625,0.0010471846,0.0002792005,0.3010342,0.00017682594,0.00029446857,0.01263181],"study_design_scores_gemma":[0.000004779587,0.00013681581,0.9844603,0.0000074413733,0.000023447601,0.0014185943,0.00023655778,0.0001931719,0.01245076,0.000035908593,0.0010228836,0.000009250241],"about_ca_topic_score_codex":0.006133861,"about_ca_topic_score_gemma":0.009366804,"teacher_disagreement_score":0.006133861,"about_ca_system_score_codex":0.00021523962,"about_ca_system_score_gemma":0.00008743109,"threshold_uncertainty_score":0.012196302},"labels":[],"label_agreement":null},{"id":"W2073925265","doi":"10.1086/522776","title":"Evidence for a Population of High‐Redshift Submillimeter Galaxies from Interferometric Imaging","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy; Luminous infrared galaxy; Radio galaxy; Astronomy; Submillimeter Array; Population; Angular resolution (graph drawing); Flux (metallurgy); Star formation","score_opus":0.018855321311024284,"score_gpt":0.25534511529372006,"score_spread":0.23648979398269576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073925265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99824893,0.00011774152,0.00060798286,0.000042401258,0.0000044500357,0.000013745274,0.00013583162,0.00002156825,0.0008074222],"genre_scores_gemma":[0.9988141,0.000044824286,0.00044863485,0.0000784236,0.000017207429,0.000009623594,0.00044160947,0.00000670521,0.00013878298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99941576,0.000058953992,0.000039518436,0.00016808818,0.00014160438,0.00017598328],"domain_scores_gemma":[0.99771166,0.00046766212,0.0007954305,0.00038912162,0.00023593937,0.00040016463],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096863374,0.00030946865,0.00047251716,0.0023233835,0.00065649796,0.0018929042,0.0009677836,0.00052322855,0.0021565454],"category_scores_gemma":[0.0020755779,0.00046901876,0.00024380168,0.0013655494,0.0011313813,0.0005464481,0.0014537825,0.00044829832,0.0004956798],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007820847,0.000058177273,0.9811544,0.000013836142,0.000039152354,0.00009517202,0.00060068537,0.00004332423,0.013219245,0.0003036364,0.00015779723,0.0042363717],"study_design_scores_gemma":[0.0000070221927,0.00003681981,0.99865913,0.0000023769173,0.000013307098,0.0002535114,0.00013412202,0.00013278899,0.0004227715,0.00011255348,0.00022129547,0.000004198961],"about_ca_topic_score_codex":0.002260146,"about_ca_topic_score_gemma":0.004648937,"teacher_disagreement_score":0.0023233835,"about_ca_system_score_codex":0.0003344737,"about_ca_system_score_gemma":0.00016419862,"threshold_uncertainty_score":0.007214427},"labels":[],"label_agreement":null},{"id":"W2073948499","doi":"10.1086/499154","title":"Disk Evolution since<i>z</i> ∼ 1 in a CDM Universe","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Astrophysics; Physics; Galaxy; Redshift; Galaxy formation and evolution; Cosmology; Astronomy; Universe; Luminosity; Peculiar galaxy; Galaxy group","score_opus":0.0038829863081109727,"score_gpt":0.18413601808991095,"score_spread":0.18025303178179997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073948499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99915326,0.00006319845,0.00010250131,0.00005653706,0.0000014786295,0.0000025331528,0.00008506804,0.000017846267,0.00051764434],"genre_scores_gemma":[0.9992046,0.000069732094,0.00028510217,0.000026318361,0.000001959994,0.0000023429577,0.00015755351,0.000005852271,0.0002467182],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999273,0.000014394575,0.0000039191646,0.000023146848,0.000010021195,0.000021177693],"domain_scores_gemma":[0.9996506,0.000076840464,0.000093407296,0.000029295588,0.000039684997,0.00011013083],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002813243,0.00024389282,0.00024435765,0.00040294378,0.00047229204,0.0010865658,0.0004522402,0.000779998,0.00089398975],"category_scores_gemma":[0.0014877779,0.00029565478,0.00024442197,0.00038821634,0.00053291814,0.00052675616,0.000448178,0.00054854306,0.00017769582],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005601013,0.0002601781,0.78592515,0.000081713755,0.00012319774,0.0007138353,0.0008431797,0.15424088,0.03376531,0.008202287,0.0015074011,0.013776777],"study_design_scores_gemma":[0.00018332058,0.0002313803,0.74343944,0.000029603798,0.00015022354,0.00047916465,0.00043411372,0.24111097,0.007234602,0.0038420404,0.0028123436,0.00005278978],"about_ca_topic_score_codex":0.018064527,"about_ca_topic_score_gemma":0.0116010085,"teacher_disagreement_score":0.018064527,"about_ca_system_score_codex":0.001554914,"about_ca_system_score_gemma":0.00030022598,"threshold_uncertainty_score":0.035918772},"labels":[],"label_agreement":null},{"id":"W2073987902","doi":"10.1088/0004-637x/788/2/158","title":"TEST OF MODELS OF THE COSMIC INFRARED BACKGROUND WITH MULTIWAVELENGTH OBSERVATIONS OF THE BLAZAR 1ES 1218+30.4 IN 2009","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Extragalactic background light; Blazar; Fermi Gamma-ray Space Telescope; Astrophysics; Spitzer Space Telescope; Redshift; Astronomy; Telescope; Active galactic nucleus; Gamma ray; Galaxy","score_opus":0.01693134401378918,"score_gpt":0.2100147457086779,"score_spread":0.19308340169488872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2073987902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9912021,0.00020950452,0.0038054204,0.0004934791,0.000020364916,0.000023090715,0.0006717235,0.00019496221,0.0033794474],"genre_scores_gemma":[0.9974396,0.000059322985,0.0009919574,0.000060530423,0.000020705253,0.000013220776,0.00089436164,0.0000838522,0.00043645062],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9990101,0.00038521673,0.000050033042,0.00032270583,0.000086239204,0.00014571942],"domain_scores_gemma":[0.9922315,0.00452971,0.001580849,0.0006435284,0.00043597637,0.0005783675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004018123,0.0010042642,0.0007952857,0.00075962854,0.00047423117,0.0019910054,0.002005407,0.0008980762,0.0021146748],"category_scores_gemma":[0.009485959,0.00050031324,0.0008315968,0.0006230343,0.00068825996,0.0012739841,0.0008130764,0.00067030865,0.00038279718],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002261482,0.0004531845,0.45066127,0.00018733321,0.0009731143,0.0008323872,0.00075469806,0.4959129,0.007421527,0.0202217,0.0035232184,0.016797151],"study_design_scores_gemma":[0.00024479625,0.00019634698,0.11230484,0.000029165734,0.0001225658,0.00008969467,0.00015592642,0.87993735,0.0009723928,0.004828952,0.0010634104,0.000054652177],"about_ca_topic_score_codex":0.033615503,"about_ca_topic_score_gemma":0.020464994,"teacher_disagreement_score":0.033615503,"about_ca_system_score_codex":0.0021397176,"about_ca_system_score_gemma":0.00071838294,"threshold_uncertainty_score":0.066839695},"labels":[],"label_agreement":null},{"id":"W2074094455","doi":"10.1086/497331","title":"The Gemini Deep Deep Survey. VII. The Redshift Evolution of the Mass‐Metallicity Relation","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":489,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Metallicity; Galaxy; Stellar mass; Redshift; Astronomy; Galaxy formation and evolution; Star formation","score_opus":0.0070324307355851155,"score_gpt":0.20578082923034466,"score_spread":0.19874839849475953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074094455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8885226,0.0023074285,0.0019816146,0.0009844126,0.000058405694,0.000071087685,0.09638931,0.00041833863,0.00926681],"genre_scores_gemma":[0.92034584,0.00043352103,0.0069218385,0.00026715436,0.00006342556,0.00005511023,0.065665275,0.00006306824,0.0061847866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967587,0.00006410762,0.000014539377,0.00008720606,0.000079192774,0.000078999896],"domain_scores_gemma":[0.9988072,0.00008206221,0.0003719263,0.00018493744,0.00028725466,0.00026649385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009150116,0.00032852034,0.00023039819,0.0014764997,0.00043125768,0.00055398437,0.00042347342,0.00035249657,0.0015727661],"category_scores_gemma":[0.0012796109,0.00016964886,0.0002443786,0.0016655354,0.00015775605,0.0003645873,0.0007731215,0.00028303073,0.0008325204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001758604,0.000025901318,0.97420937,0.000040482853,0.000082983235,0.00005989058,0.0002643159,0.00017726049,0.0023232524,0.00053890113,0.007419989,0.014681824],"study_design_scores_gemma":[0.000006182863,0.000013484153,0.98959804,0.000004130948,0.00001227306,0.00003068515,0.000047180576,0.00020049709,0.00041363804,0.00005129566,0.00961919,0.0000033732313],"about_ca_topic_score_codex":0.19548796,"about_ca_topic_score_gemma":0.29897794,"teacher_disagreement_score":0.19548796,"about_ca_system_score_codex":0.001739944,"about_ca_system_score_gemma":0.00056658237,"threshold_uncertainty_score":0.38870025},"labels":[],"label_agreement":null},{"id":"W2074107843","doi":"10.1086/424560","title":"A New Classical T Tauri Object at the Substellar Boundary in Chamaeleon II","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; T Tauri star; Brown dwarf; Stars; Protostar; Stellar classification; Photometry (optics); Spectral line; Astronomy; Accretion (finance); Molecular cloud; Sky; Star formation","score_opus":0.008319512349563237,"score_gpt":0.22826555516330377,"score_spread":0.21994604281374053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074107843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988657,0.00003527949,0.00010779782,0.000013737447,0.0000016573503,0.0000029641956,0.000042169126,0.00000786071,0.00092280237],"genre_scores_gemma":[0.9992366,0.000014862042,0.00025999072,0.000015605945,0.0000040705104,0.000001961656,0.00016954358,0.000002514726,0.0002949387],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998299,0.000010709593,0.0000066814064,0.00006267644,0.000035697554,0.00005424193],"domain_scores_gemma":[0.9995869,0.000042788724,0.000107247055,0.00006543032,0.00005302855,0.00014462986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021197811,0.000261898,0.00027109284,0.0011280795,0.0014974667,0.0009215275,0.00031229918,0.00045302243,0.0013733662],"category_scores_gemma":[0.00051528536,0.00015934314,0.00011553983,0.000820586,0.00042805154,0.00038843992,0.00070134114,0.00023181854,0.0003404704],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050007744,0.00007983304,0.85112596,0.00004471387,0.000044580982,0.0037118737,0.0023342997,0.00029616884,0.12023809,0.0009104122,0.00041544434,0.020298434],"study_design_scores_gemma":[0.000010444618,0.00013474248,0.98965377,0.0000067125297,0.000014671583,0.0024310513,0.00046626216,0.0004907988,0.004155678,0.00017907516,0.0024463136,0.000010442218],"about_ca_topic_score_codex":0.0078198165,"about_ca_topic_score_gemma":0.013267239,"teacher_disagreement_score":0.0078198165,"about_ca_system_score_codex":0.00045879697,"about_ca_system_score_gemma":0.00017464573,"threshold_uncertainty_score":0.015548646},"labels":[],"label_agreement":null},{"id":"W2074187822","doi":"10.1088/0004-637x/701/1/587","title":"A DEEP<i>HUBBLE SPACE TELESCOPE</i><i>H</i>-BAND IMAGING SURVEY OF MASSIVE GAS-RICH MERGERS. II. THE QUEST QSOs","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"QSOS; Physics; Astrophysics; Astronomy; Luminosity; Quasar; Hubble space telescope; Galaxy","score_opus":0.006446952309710915,"score_gpt":0.21430383301426006,"score_spread":0.20785688070454916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074187822","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9923308,0.00027322958,0.00030492622,0.00003499884,0.0000026769505,0.000024075214,0.0048746127,0.000041949173,0.0021126762],"genre_scores_gemma":[0.9784934,0.00024043799,0.0017675448,0.00007730604,0.000023210017,0.000025240917,0.017692575,0.000019794034,0.0016605386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987054,0.000011724452,0.000007079139,0.000037986065,0.000027029151,0.000045681107],"domain_scores_gemma":[0.99950695,0.000024739407,0.00017164448,0.000042248546,0.00004952945,0.00020481455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022877417,0.00026443467,0.00018215354,0.0026749263,0.00022973768,0.00039759933,0.00016815001,0.00012151326,0.0017243064],"category_scores_gemma":[0.00020356823,0.00011980174,0.0001819076,0.0010848535,0.00022995881,0.00030327513,0.00062594895,0.00014409763,0.00053613784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000100611265,0.000063723994,0.958916,0.000040034407,0.000046509824,0.00015458542,0.00032218135,0.00013635287,0.02527448,0.00034514122,0.0017369792,0.012863434],"study_design_scores_gemma":[0.000004742907,0.000028637098,0.99719954,0.000002772535,0.000008344727,0.00014412834,0.00005500392,0.000080797254,0.00059427466,0.000032274504,0.0018473982,0.0000019922645],"about_ca_topic_score_codex":0.0047293385,"about_ca_topic_score_gemma":0.014312793,"teacher_disagreement_score":0.0047293385,"about_ca_system_score_codex":0.0003249621,"about_ca_system_score_gemma":0.00026607042,"threshold_uncertainty_score":0.009403586},"labels":[],"label_agreement":null},{"id":"W2074226175","doi":"10.1088/0004-637x/758/1/41","title":"STELLAR POPULATIONS AND RADIAL MIGRATIONS IN VIRGO DISK GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Virgo Cluster; Galaxy; Interacting galaxy; Lenticular galaxy; Galaxy cluster; Cluster (spacecraft); Brightest cluster galaxy; Luminosity; Galaxy merger","score_opus":0.012059620146253058,"score_gpt":0.2275023728330208,"score_spread":0.21544275268676774,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074226175","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995598,0.000044012446,0.00005770356,0.0000038745748,2.8604643e-7,7.414125e-7,0.00009596357,0.0000068910567,0.00023063445],"genre_scores_gemma":[0.9995009,0.000024514076,0.00010539197,0.0000020986777,6.0251705e-7,0.0000011973311,0.00020893577,0.000002064364,0.00015426172],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999418,0.00000858817,0.000003496662,0.000020657644,0.000007692242,0.000017678825],"domain_scores_gemma":[0.99953103,0.00010009635,0.00013349917,0.00006169581,0.00007303893,0.000100701865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002343165,0.00013593091,0.0001147134,0.0017024801,0.00018864592,0.00040524703,0.00018325506,0.0002207002,0.0007924213],"category_scores_gemma":[0.0010324026,0.00008472706,0.00012768782,0.00051946996,0.0002172855,0.00020616205,0.0003557995,0.00011468343,0.00026738134],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013096422,0.00001701309,0.98377454,0.00000854363,0.000024722664,0.000048148824,0.00039405315,0.0027878855,0.007574451,0.00037890443,0.00008064118,0.004780024],"study_design_scores_gemma":[0.0000018656617,0.000023587581,0.99643564,0.0000028342279,0.0000057541442,0.00006682392,0.00014549325,0.002415828,0.0005316545,0.00015317171,0.00021304496,0.0000042316146],"about_ca_topic_score_codex":0.0056600054,"about_ca_topic_score_gemma":0.0061109997,"teacher_disagreement_score":0.0056600054,"about_ca_system_score_codex":0.0003997203,"about_ca_system_score_gemma":0.00008096887,"threshold_uncertainty_score":0.011254132},"labels":[],"label_agreement":null},{"id":"W2074274881","doi":"10.1088/0004-637x/701/2/1814","title":"A BACKWARD EVOLUTION MODEL FOR INFRARED SURVEYS: THE ROLE OF AGN– AND COLOR–<i>L</i><sub>TIR</sub>DISTRIBUTIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Luminous infrared galaxy; Luminosity; Luminosity function; Galaxy formation and evolution; Infrared; Spectral energy distribution; Astronomy; Star formation","score_opus":0.007188813661920537,"score_gpt":0.2070366770007528,"score_spread":0.19984786333883225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074274881","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.10593969,0.00040965082,0.8885324,0.0006502303,0.000041333275,0.00009944618,0.00072807225,0.00044278277,0.003156428],"genre_scores_gemma":[0.78035957,0.0011578049,0.19104068,0.000575928,0.00015510747,0.0007068807,0.0019370695,0.00063092395,0.023436105],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990847,0.0003886034,0.000032596094,0.00026058313,0.000117652235,0.000115774754],"domain_scores_gemma":[0.9963696,0.00213365,0.0006046212,0.0003534839,0.0003929613,0.00014577166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0040679504,0.000943209,0.0009598808,0.0013534146,0.00075753254,0.0017030387,0.0039620595,0.0016793957,0.0030965232],"category_scores_gemma":[0.0094783055,0.0013265219,0.0015090219,0.001176868,0.0013441433,0.002926121,0.0013647524,0.0016368265,0.00095197547],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000094609124,0.00004823685,0.027376799,0.000080841404,0.00012368009,0.00022254328,0.00034352433,0.8008756,0.0024715196,0.14983644,0.001349047,0.017177194],"study_design_scores_gemma":[0.000010478656,0.00001420477,0.0013655112,0.000010347098,0.000021342054,0.00008394489,0.000011414377,0.97877216,0.00024347872,0.018481087,0.00096953433,0.000016526199],"about_ca_topic_score_codex":0.02130994,"about_ca_topic_score_gemma":0.013616492,"teacher_disagreement_score":0.02130994,"about_ca_system_score_codex":0.0020841842,"about_ca_system_score_gemma":0.0012129211,"threshold_uncertainty_score":0.04237181},"labels":[],"label_agreement":null},{"id":"W2074281376","doi":"10.1086/498143","title":"Raman‐scattered He<scp>ii</scp>λλ4850, 6545 in the Young and Compact Planetary Nebula IC 5117","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Nebula; Raman scattering; Raman spectroscopy; Stars; Astrophysics; Planetary nebula; Scattering; Emission spectrum; Spectral line; Astronomy; Optics","score_opus":0.008181996451691839,"score_gpt":0.21588798883340513,"score_spread":0.20770599238171328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074281376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991566,0.00007720933,0.00035362397,0.0000063547895,0.0000014703688,0.0000020723464,0.000034819765,0.0000119187425,0.00035607387],"genre_scores_gemma":[0.99957687,0.000030611864,0.00023784893,0.0000039570346,0.0000019237323,0.0000019220947,0.00006403431,0.0000034391378,0.000079454374],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999273,0.000004491511,0.0000023107993,0.000024086248,0.000021316433,0.00002052121],"domain_scores_gemma":[0.9998883,0.000023976085,0.000034194018,0.000016276183,0.0000130904855,0.000024154593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017535106,0.00032842642,0.00015785024,0.00049108505,0.00027483513,0.0004244897,0.00040150186,0.00019684013,0.00040923632],"category_scores_gemma":[0.0002580539,0.00021544166,0.0002919621,0.0003391215,0.00035743203,0.00019140192,0.00027080686,0.00015042734,0.00013116418],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002666856,0.00007414616,0.7393928,0.00006638197,0.0001914235,0.0024864934,0.00041659994,0.013645035,0.23061115,0.0013106749,0.0002748655,0.011263876],"study_design_scores_gemma":[0.000029670613,0.00013175167,0.94834495,0.000011813213,0.000060487306,0.0008465137,0.00019151208,0.023500094,0.02553435,0.0005005561,0.0008284383,0.000019920535],"about_ca_topic_score_codex":0.004393365,"about_ca_topic_score_gemma":0.0053060334,"teacher_disagreement_score":0.004393365,"about_ca_system_score_codex":0.0004906172,"about_ca_system_score_gemma":0.00015120722,"threshold_uncertainty_score":0.008735597},"labels":[],"label_agreement":null},{"id":"W2074314047","doi":"10.1086/324437","title":"A High Spatial Resolution Analysis of the MAXIMA-1 Cosmic Microwave Background Anisotropy Data","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":396,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Maxima; Cosmic microwave background; Astrophysics; Amplitude; Range (aeronautics); Bolometer; Cosmic background radiation; Sky; Angular resolution (graph drawing); Multipole expansion; Anisotropy; Astronomy; Optics; Detector","score_opus":0.019784672610141656,"score_gpt":0.26462142161284835,"score_spread":0.2448367490027067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074314047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96017367,0.0006034594,0.02235433,0.00035001128,0.000033532353,0.000035028712,0.0056553213,0.0006244099,0.010170277],"genre_scores_gemma":[0.96193767,0.00027940303,0.029170604,0.000054341435,0.000101414786,0.000035542133,0.0070152404,0.00017268058,0.0012332037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996093,0.00007268497,0.0000122461515,0.00008788686,0.00014390542,0.00007394467],"domain_scores_gemma":[0.9992086,0.00015973946,0.0001305252,0.00027152104,0.00014251897,0.00008706827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005507153,0.00023761309,0.00031389343,0.0017927241,0.00030046594,0.0006325847,0.0003118951,0.00017430152,0.0010057329],"category_scores_gemma":[0.0011476185,0.0001798849,0.0005172816,0.0015815693,0.0001773157,0.00034589035,0.0007427329,0.0006069998,0.00044517088],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094592903,0.00032957995,0.5025081,0.0002733312,0.00083258067,0.0017788912,0.00084190414,0.030113347,0.10931342,0.01478269,0.015209284,0.323071],"study_design_scores_gemma":[0.00005068043,0.000058379013,0.9498669,0.000019824723,0.00008521227,0.00047561547,0.0001214174,0.019962441,0.010618754,0.0020907903,0.01660367,0.00004630473],"about_ca_topic_score_codex":0.004180997,"about_ca_topic_score_gemma":0.006600369,"teacher_disagreement_score":0.004180997,"about_ca_system_score_codex":0.0002686188,"about_ca_system_score_gemma":0.00023752701,"threshold_uncertainty_score":0.008313298},"labels":[],"label_agreement":null},{"id":"W2074347757","doi":"10.1088/0004-637x/770/2/103","title":"THE<i>NUCLEAR SPECTROSCOPIC TELESCOPE ARRAY</i>(<i>NuSTAR</i>) HIGH-ENERGY X-RAY MISSION","year":2013,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2267,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Quest University Canada; McGill University","funders":"Lawrence Livermore National Laboratory; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Leverhulme Trust; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; Killam Trusts; Fonds Québécois de la Recherche sur la Nature et les Technologies; Centre National d’Etudes Spatiales; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Telescope; X-ray telescope; Astronomy; X-ray astronomy; Astrophysics; X-ray; Nuclear physics","score_opus":0.00790922814067132,"score_gpt":0.20724087001377908,"score_spread":0.19933164187310776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074347757","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07026222,0.008968151,0.012364215,0.027815452,0.002489012,0.00021998063,0.04972525,0.0047813538,0.82337445],"genre_scores_gemma":[0.53850925,0.012831442,0.07595356,0.006405062,0.002463973,0.0002932293,0.0809651,0.0022423505,0.28033608],"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9994599,0.000098216544,0.000019891828,0.000101909645,0.0002630384,0.000056999874],"domain_scores_gemma":[0.99817336,0.00016850012,0.0003321154,0.00029594277,0.0005648797,0.0004652238],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016370051,0.00022023795,0.00022465872,0.0014283927,0.0011072715,0.0024117713,0.00043813893,0.0005047606,0.015482468],"category_scores_gemma":[0.0023647826,0.0001259191,0.00016747555,0.0019105923,0.0004751062,0.00200853,0.0021221815,0.0008571134,0.0035610385],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004534729,0.00017248961,0.04888715,0.00051703793,0.00008904155,0.00020712792,0.0011784541,0.0005199707,0.015875617,0.07021008,0.52760816,0.3342814],"study_design_scores_gemma":[0.000024714245,0.0000263979,0.02342354,0.00008454178,0.000013056448,0.00008962332,0.00027133443,0.00027427584,0.0017558726,0.0036089877,0.9704123,0.000015202327],"about_ca_topic_score_codex":0.015086098,"about_ca_topic_score_gemma":0.028321696,"teacher_disagreement_score":0.015482468,"about_ca_system_score_codex":0.001610621,"about_ca_system_score_gemma":0.0033846581,"threshold_uncertainty_score":0.051793993},"labels":[],"label_agreement":null},{"id":"W2074435279","doi":"10.1088/0004-637x/756/2/179","title":"DYNAMICAL MEASUREMENTS OF BLACK HOLE MASSES IN FOUR BRIGHTEST CLUSTER GALAXIES AT 100 Mpc","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Australian Research Council; Ministerio de Ciencia, Tecnología e Innovación Productiva; Science and Technology Facilities Council; Cynthia and George Mitchell Foundation; Ministério da Ciência e Tecnologia; W. M. Keck Foundation; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Velocity dispersion; Stellar kinematics; Astronomy; Black hole (networking); Dark matter; Luminosity; RADIUS; Dark matter halo; Stellar mass; Halo; Milky Way; Star formation","score_opus":0.018215845576968384,"score_gpt":0.23209812092087595,"score_spread":0.21388227534390758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074435279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999539,0.000011518591,0.00015583159,0.0000035078865,3.60675e-7,0.0000017132144,0.00009023151,0.000019044357,0.00017888447],"genre_scores_gemma":[0.99895763,0.0000119523465,0.00051668176,0.0000021532705,0.0000014969421,0.0000026664407,0.000402031,0.0000038553203,0.000101505844],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990344,0.000009249273,0.0000035595892,0.000031911924,0.000023960309,0.000027878174],"domain_scores_gemma":[0.99949884,0.00008714956,0.00015200095,0.000070247836,0.00005849795,0.00013324965],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018146739,0.0003292685,0.0001880924,0.00090267754,0.0004514924,0.00026936075,0.0005458005,0.00023213572,0.00079340016],"category_scores_gemma":[0.00062419125,0.0002186159,0.00023266509,0.0003790267,0.00031832047,0.00025514772,0.00047704283,0.00019927905,0.00018783844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017846187,0.0000508559,0.9763781,0.000009949741,0.00004670571,0.000076325116,0.00031125723,0.0033050543,0.014193756,0.00025002545,0.0001756939,0.0050239],"study_design_scores_gemma":[0.0000137455045,0.00006614052,0.98370516,0.0000019391769,0.000021071004,0.00007329213,0.000064657375,0.0120975515,0.0035269498,0.00012834508,0.00029033833,0.000010829534],"about_ca_topic_score_codex":0.0140308505,"about_ca_topic_score_gemma":0.022081954,"teacher_disagreement_score":0.0140308505,"about_ca_system_score_codex":0.0008829214,"about_ca_system_score_gemma":0.00011263637,"threshold_uncertainty_score":0.027898371},"labels":[],"label_agreement":null},{"id":"W2074464944","doi":"10.1088/0004-637x/718/2/632","title":"ANGULAR POWER SPECTRA OF THE MILLIMETER-WAVELENGTH BACKGROUND LIGHT FROM DUSTY STAR-FORMING GALAXIES WITH THE SOUTH POLE TELESCOPE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":146,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; Office of Polar Programs; McGill University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Gordon and Betty Moore Foundation; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Emissivity; South Pole Telescope; Telescope; Amplitude; Redshift; Spectral index; Spectral density; Context (archaeology); Astronomy; Cosmic microwave background; Spectral line; Anisotropy; Optics","score_opus":0.006004311366738418,"score_gpt":0.18964598336457458,"score_spread":0.18364167199783615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074464944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98371106,0.00095413293,0.002931587,0.0006610923,0.000053746346,0.000014835321,0.0027273924,0.0004407856,0.008505384],"genre_scores_gemma":[0.993654,0.00033464443,0.0008784114,0.000084106054,0.00007560163,0.000010487147,0.0035735227,0.00011273153,0.0012765595],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997564,0.000034668217,0.000009491585,0.000052310563,0.00010675468,0.000040253668],"domain_scores_gemma":[0.99886644,0.00030486006,0.00024331886,0.000101163954,0.00024840367,0.00023586692],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039691292,0.000458283,0.00028051247,0.0014299633,0.00024996765,0.00064824533,0.00029785052,0.0003510661,0.0022872407],"category_scores_gemma":[0.0013780429,0.00032241008,0.00035573065,0.0013305919,0.00017070716,0.00039151649,0.0006026504,0.0005847522,0.00081682095],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017725722,0.00014562721,0.8251199,0.0001772196,0.00046141548,0.0008469923,0.0007736387,0.004050893,0.10970619,0.0016639092,0.010660215,0.04462148],"study_design_scores_gemma":[0.000011787185,0.000017178343,0.99667704,0.000004588934,0.000030251518,0.0001161994,0.000024627687,0.00090090523,0.0012695232,0.00008608475,0.0008555841,0.0000062838367],"about_ca_topic_score_codex":0.004170425,"about_ca_topic_score_gemma":0.0063062585,"teacher_disagreement_score":0.004170425,"about_ca_system_score_codex":0.00056671177,"about_ca_system_score_gemma":0.00017220927,"threshold_uncertainty_score":0.008292258},"labels":[],"label_agreement":null},{"id":"W2074492627","doi":"10.1086/430466","title":"Properties of Extremely Red Objects in an Overdense Region","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Field (mathematics); Astrophysics; Physics; Population; Normalization (sociology); Mathematics","score_opus":0.017386808594771933,"score_gpt":0.21212282046982847,"score_spread":0.19473601187505654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074492627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747795,0.00012972667,0.00016631868,0.000017728244,0.000001347135,0.000003878323,0.00029569652,0.00001862479,0.0018888381],"genre_scores_gemma":[0.9987978,0.000041755808,0.00015816533,0.000012102815,0.000004489313,0.0000029730247,0.00048083588,0.0000050472345,0.0004967615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989426,0.000011956071,0.000006242488,0.000034545268,0.000023066113,0.000029943118],"domain_scores_gemma":[0.9992077,0.0001602778,0.00025119976,0.00008103467,0.00013197516,0.00016781743],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020813677,0.00010749953,0.00017956273,0.0016753529,0.0004355494,0.00058047415,0.00022578891,0.00028448648,0.0020774868],"category_scores_gemma":[0.0007990429,0.00012408472,0.00010774296,0.0014344184,0.00024784746,0.00037650488,0.00046483363,0.00016875457,0.00042735573],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023647606,0.00004476083,0.97796965,0.000017108017,0.000039093655,0.00020480681,0.00034504707,0.00050050666,0.008805146,0.0004105321,0.0005284443,0.010898324],"study_design_scores_gemma":[0.000001885531,0.0000145809645,0.99831164,0.000002745415,0.000010253111,0.00020126098,0.00018690103,0.00038883148,0.00026044063,0.0001043519,0.0005143478,0.0000028806437],"about_ca_topic_score_codex":0.008986843,"about_ca_topic_score_gemma":0.0090453895,"teacher_disagreement_score":0.008986843,"about_ca_system_score_codex":0.00022271536,"about_ca_system_score_gemma":0.000089866386,"threshold_uncertainty_score":0.017869055},"labels":[],"label_agreement":null},{"id":"W2074535692","doi":"10.1086/590344","title":"Conduction and the Star Formation Threshold in Brightest Cluster Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Star formation; Luminosity function; Astronomy; Galaxy cluster; Galaxy; Luminosity; Intracluster medium","score_opus":0.011046189993767844,"score_gpt":0.2042125582191285,"score_spread":0.19316636822536065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074535692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989723,0.00011980579,0.00006714006,0.000052632993,0.0000010104709,6.465041e-7,0.000017746339,0.000010696305,0.00075811386],"genre_scores_gemma":[0.9998448,0.000018690649,0.000021850476,0.000008854563,0.0000021264818,3.5988634e-7,0.000018747738,0.0000018656818,0.000082655904],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9998895,0.00001553021,0.0000053382964,0.000020377975,0.000011877223,0.000057258265],"domain_scores_gemma":[0.99801254,0.0005292098,0.0005158765,0.000100079924,0.000105123196,0.00073708885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040864162,0.00009197538,0.00026945912,0.00092128356,0.0004951445,0.001414655,0.00027340636,0.00036835426,0.0014956169],"category_scores_gemma":[0.0022129137,0.00014700151,0.000110036875,0.0003219598,0.00094967167,0.0005013181,0.0006939648,0.00039511351,0.00021082758],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004609627,0.00007799999,0.9675694,0.000026024294,0.000021285872,0.00022791601,0.0011758994,0.0014711105,0.014600089,0.007371026,0.00034309097,0.00665512],"study_design_scores_gemma":[0.000022130902,0.00004420243,0.98720586,0.0000085382135,0.000011061489,0.0002048843,0.00035867572,0.0014860982,0.0015551846,0.008724365,0.0003709657,0.00000801026],"about_ca_topic_score_codex":0.0042831944,"about_ca_topic_score_gemma":0.0031049703,"teacher_disagreement_score":0.0042831944,"about_ca_system_score_codex":0.00078323163,"about_ca_system_score_gemma":0.00028433357,"threshold_uncertainty_score":0.00851649},"labels":[],"label_agreement":null},{"id":"W2074571975","doi":"10.1086/511810","title":"Resonant Cyclotron Scattering in Three Dimensions and the Quiescent Nonthermal X‐ray Emission of Magnetars","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Magnetar; Scattering; Spectral line; Cyclotron; Magnetic field; Photon; Emission spectrum; Thermal","score_opus":0.009166449549357398,"score_gpt":0.287082568120336,"score_spread":0.2779161185709786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074571975","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993331,0.00004231628,0.0054162876,0.000019237064,0.0000028576853,0.0000054597413,0.000034526343,0.00005845302,0.0010897334],"genre_scores_gemma":[0.9985738,0.000025378082,0.0011874889,0.0000038209755,0.000001405157,0.0000045758393,0.000041742744,0.000013841025,0.00014793794],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999559,0.000009824237,0.0000025111494,0.000008760436,0.000011446778,0.0000115859075],"domain_scores_gemma":[0.99983335,0.00007386136,0.000041144824,0.00001657862,0.000018284043,0.000016832504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015190609,0.00020250058,0.00009184085,0.0002995932,0.00020309187,0.0005132193,0.00023418917,0.00017907475,0.0005607658],"category_scores_gemma":[0.0004408075,0.0001754693,0.0003232984,0.00021685522,0.0003129886,0.00018673127,0.00018583518,0.00016249003,0.00006893917],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004095811,0.00016719675,0.05471724,0.000073004056,0.00009145232,0.00079624687,0.00047424686,0.68033975,0.22626483,0.025538713,0.00029915923,0.010828611],"study_design_scores_gemma":[0.00005530075,0.00012127918,0.054279167,0.000009751225,0.00002120067,0.0002596591,0.000115967574,0.90685755,0.033543024,0.0042179064,0.00048402502,0.000035248308],"about_ca_topic_score_codex":0.0017612509,"about_ca_topic_score_gemma":0.0008119092,"teacher_disagreement_score":0.0017612509,"about_ca_system_score_codex":0.0004392335,"about_ca_system_score_gemma":0.00016021884,"threshold_uncertainty_score":0.0035020113},"labels":[],"label_agreement":null},{"id":"W2074585149","doi":"10.1086/340229","title":"Spectral Components of the Radio Composite Supernova Remnant G11.2−0.3","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar wind nebula; Spectral index; Physics; Supernova remnant; Astrophysics; Pulsar; Supernova; Astronomy; Spectral line","score_opus":0.013578271802400826,"score_gpt":0.2040021428222151,"score_spread":0.19042387101981428,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074585149","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988318,0.0001145201,0.0003739749,0.000004544956,0.0000012992541,0.000003102928,0.00016813885,0.000027433496,0.00047524765],"genre_scores_gemma":[0.997931,0.00006304281,0.00078370667,0.000007732514,0.000005456252,0.000003978194,0.00095918233,0.000013655734,0.00023223064],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999664,0.0000028544443,0.0000018425882,0.000012413528,0.000008156417,0.000008485222],"domain_scores_gemma":[0.9997892,0.000027945629,0.00007395698,0.00002976633,0.000028355273,0.00005079059],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013946561,0.00022518929,0.00015436,0.00084081327,0.00015197505,0.00031739016,0.0002132258,0.000111658526,0.0007579615],"category_scores_gemma":[0.00020557083,0.0001359103,0.00018758,0.00043342385,0.00014207362,0.00014419935,0.00027877657,0.00014537686,0.00027612288],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014415504,0.00020441167,0.5343078,0.000108601256,0.00019228959,0.002207406,0.00042058146,0.0025816977,0.42755446,0.00079778855,0.0006710837,0.02951229],"study_design_scores_gemma":[0.0000127527655,0.00015417248,0.98876137,0.000003651649,0.00003725652,0.0015213486,0.000052418643,0.002153451,0.006484652,0.00012581871,0.00068169436,0.000011366172],"about_ca_topic_score_codex":0.001275212,"about_ca_topic_score_gemma":0.0021743483,"teacher_disagreement_score":0.001275212,"about_ca_system_score_codex":0.00012682177,"about_ca_system_score_gemma":0.000046400044,"threshold_uncertainty_score":0.0025356412},"labels":[],"label_agreement":null},{"id":"W2074620144","doi":"10.1088/0004-637x/777/2/168","title":"BROAD ABSORPTION LINE VARIABILITY ON MULTI-YEAR TIMESCALES IN A LARGE QUASAR SAMPLE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":149,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Astrophysics; Trough (economics); Sky; Physics; Galaxy","score_opus":0.010219890909582433,"score_gpt":0.2309932911418241,"score_spread":0.22077340023224168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074620144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99919397,0.00010055584,0.00007030568,0.000032273525,0.0000020494206,0.000001943623,0.00032373355,0.00000805793,0.0002671402],"genre_scores_gemma":[0.9992532,0.0000362097,0.00006299403,0.000013535444,0.0000062361596,0.000003064247,0.00038257093,0.0000035604648,0.00023874239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988055,0.000016436348,0.000006763319,0.00005082348,0.000018855979,0.00002659535],"domain_scores_gemma":[0.99934,0.000112357295,0.0002445579,0.000067045934,0.00009503692,0.00014090288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033326258,0.00006861242,0.00013502187,0.00095810276,0.0002740269,0.00049923826,0.00021757244,0.00021857941,0.0011993959],"category_scores_gemma":[0.0007329241,0.0000976895,0.0001241363,0.0006400922,0.00018305858,0.0003285395,0.00044344584,0.00024281972,0.00022301538],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006599236,0.00005402226,0.9851317,0.000007271358,0.000056286288,0.00008107514,0.00036922426,0.00008180255,0.0043293983,0.000091707254,0.00048311008,0.009248463],"study_design_scores_gemma":[7.5054356e-7,0.0000071236827,0.9995771,6.673996e-7,0.0000040901514,0.000033302695,0.00007671854,0.00005876164,0.00003449744,0.000013488357,0.00019254143,9.178242e-7],"about_ca_topic_score_codex":0.009860963,"about_ca_topic_score_gemma":0.017469047,"teacher_disagreement_score":0.009860963,"about_ca_system_score_codex":0.00019338827,"about_ca_system_score_gemma":0.000101691585,"threshold_uncertainty_score":0.019607127},"labels":[],"label_agreement":null},{"id":"W2074648364","doi":"10.1088/0004-637x/745/2/119","title":"CLOSE COMPANIONS TO YOUNG STARS. I. A LARGE SPECTROSCOPIC SURVEY IN CHAMAELEON I AND TAURUS-AURIGA","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":171,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Stars; T Tauri star; Radial velocity; Planet; Astronomy; Accretion (finance); Telescope","score_opus":0.016314927308477764,"score_gpt":0.2671306378170635,"score_spread":0.2508157105085857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074648364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99850273,0.00042395803,0.00008295721,0.000012600215,0.0000023027542,0.0000039944975,0.00018114649,0.000008453787,0.00078187697],"genre_scores_gemma":[0.9987815,0.00012645047,0.00021147245,0.000011041788,0.000007742027,0.0000032445212,0.0004832272,0.000002157853,0.00037316215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979275,0.000016770724,0.000012300338,0.000078886485,0.000049559585,0.000049781323],"domain_scores_gemma":[0.99912304,0.000077088946,0.00043793902,0.00005828938,0.000053247837,0.00025043509],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023994135,0.00029637755,0.0002814614,0.0022456269,0.0007542439,0.000645024,0.0002669188,0.00024319204,0.0016701961],"category_scores_gemma":[0.00056845834,0.00012232474,0.00017338486,0.0011534578,0.00022805744,0.0004106011,0.00076372194,0.00015453805,0.00049966696],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007932942,0.00002055059,0.9833665,0.000020078902,0.000025967407,0.00025735548,0.00040474255,0.000037825437,0.008004816,0.00009477671,0.00014267142,0.0075453673],"study_design_scores_gemma":[0.0000019686995,0.000038883813,0.9977552,0.0000031417455,0.0000102240965,0.0004228814,0.00016268816,0.00004707742,0.00042713885,0.0000275914,0.0011008794,0.0000021655385],"about_ca_topic_score_codex":0.006895265,"about_ca_topic_score_gemma":0.020806277,"teacher_disagreement_score":0.006895265,"about_ca_system_score_codex":0.00045079814,"about_ca_system_score_gemma":0.00022115857,"threshold_uncertainty_score":0.01371026},"labels":[],"label_agreement":null},{"id":"W2074758955","doi":"10.1088/0004-637x/795/2/158","title":"THE MASSIVE SURVEY. I. A VOLUME-LIMITED INTEGRAL-FIELD SPECTROSCOPIC STUDY OF THE MOST MASSIVE EARLY-TYPE GALAXIES WITHIN 108 Mpc","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":216,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Supermassive black hole; Astronomy; Galaxy; Stellar mass; Dark matter; Galaxy formation and evolution; Elliptical galaxy; Star formation","score_opus":0.008221633568808784,"score_gpt":0.21974531359713334,"score_spread":0.21152368002832456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074758955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81499577,0.0020348015,0.010718403,0.0010631073,0.00012040869,0.0003572927,0.12001225,0.0017725771,0.048925348],"genre_scores_gemma":[0.8520708,0.0009784857,0.025475275,0.00080876675,0.00029583363,0.00027633773,0.105795495,0.00020491403,0.014094258],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99964833,0.00005678825,0.000015185971,0.00012390217,0.00008865864,0.00006719818],"domain_scores_gemma":[0.9988127,0.00005733608,0.00036799893,0.00020566744,0.000121627185,0.00043476146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006452835,0.00048101382,0.00026028694,0.0017183388,0.00041732495,0.00063661946,0.0004413608,0.00025726508,0.0026362238],"category_scores_gemma":[0.0008241071,0.00021529935,0.00026519262,0.0011915722,0.00022587784,0.0005865862,0.0015470749,0.0002957044,0.00156561],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044669225,0.00016694648,0.788598,0.00025420974,0.0002111871,0.0002379743,0.0006508415,0.0007689545,0.027427098,0.005253703,0.037615757,0.13836864],"study_design_scores_gemma":[0.00006341347,0.00019543774,0.9266943,0.00005739309,0.000059933176,0.00038703647,0.00019233015,0.0011187998,0.0026729875,0.0012610054,0.06728124,0.000016116528],"about_ca_topic_score_codex":0.004497022,"about_ca_topic_score_gemma":0.010535054,"teacher_disagreement_score":0.004497022,"about_ca_system_score_codex":0.00044705518,"about_ca_system_score_gemma":0.00049062417,"threshold_uncertainty_score":0.00894171},"labels":[],"label_agreement":null},{"id":"W2074778956","doi":"10.1088/0004-637x/727/1/3","title":"THE ELM SURVEY. II. TWELVE BINARY WHITE DWARF MERGER SYSTEMS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"White dwarf; Gravitational wave; Sky; Binary number; Binary star; Neutron star; Merge (version control); Orbital period","score_opus":0.010406934809453459,"score_gpt":0.22973401300094867,"score_spread":0.21932707819149522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074778956","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93610823,0.0012205081,0.0008316224,0.0002866477,0.000018191919,0.000108283704,0.052637734,0.00022602575,0.00856275],"genre_scores_gemma":[0.85246617,0.0007354795,0.0037373712,0.00039679417,0.000068998466,0.00025339113,0.13246526,0.000060448543,0.009816125],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974865,0.000039192888,0.00002875974,0.00006024705,0.000058760466,0.0000644588],"domain_scores_gemma":[0.99945015,0.000035968846,0.00022474673,0.000063636224,0.00007383065,0.00015166876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004968572,0.00023714548,0.0002078617,0.0023679908,0.00031697133,0.00037420797,0.00032350526,0.00022380633,0.0024695],"category_scores_gemma":[0.00051942765,0.0001619542,0.00014701272,0.0016805361,0.00012923441,0.00039443534,0.0010097235,0.00018110094,0.0014374363],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021537427,0.000052644657,0.9349819,0.00013559371,0.000061347426,0.00023788412,0.00040869004,0.0001214254,0.003491801,0.0004158743,0.015899548,0.043977935],"study_design_scores_gemma":[0.00002241159,0.000027002412,0.9777003,0.000016388212,0.000015103822,0.0002412133,0.00013928719,0.00015511276,0.00050837593,0.000056297828,0.02111478,0.000003681608],"about_ca_topic_score_codex":0.009894139,"about_ca_topic_score_gemma":0.023964148,"teacher_disagreement_score":0.009894139,"about_ca_system_score_codex":0.0005558724,"about_ca_system_score_gemma":0.00034889716,"threshold_uncertainty_score":0.019673109},"labels":[],"label_agreement":null},{"id":"W2074962208","doi":"10.1086/429531","title":"Simulation of Astrophysical Jets: Collimation and Expansion into Radio Lobes","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Active galactic nucleus; Supermassive black hole; Collimated light; Astrophysics; Astrophysical jet; Accretion (finance); Magnetohydrodynamics; Galaxy; Jet (fluid); Accretion disc; Astronomy; Quasar; Plasma; Optics; Mechanics; Laser","score_opus":0.00730203009931068,"score_gpt":0.23555699487501316,"score_spread":0.22825496477570248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074962208","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9435164,0.00038095025,0.045809563,0.0007085785,0.000065992914,0.000048246882,0.000359833,0.00030119185,0.008809195],"genre_scores_gemma":[0.98753905,0.00021333648,0.010510984,0.00007777834,0.00001885452,0.000048042675,0.0001969218,0.00003931685,0.0013557608],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991786,0.000028418457,0.0000049774185,0.000009905701,0.000018012333,0.000020847618],"domain_scores_gemma":[0.9993037,0.00045024016,0.00010107263,0.00003566771,0.000054717955,0.00005467888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032268284,0.00037300054,0.00040888926,0.00028072225,0.0003472248,0.00073284167,0.00072235777,0.0010324474,0.0014187942],"category_scores_gemma":[0.0014951192,0.00026343542,0.00046871597,0.00037110338,0.00064433715,0.00053114275,0.0005973098,0.0004691191,0.00011805296],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054027267,0.000041334406,0.0023715638,0.000019714416,0.000015109341,0.00006118478,0.000040575145,0.9924077,0.0009596277,0.002587675,0.00014388486,0.0012976285],"study_design_scores_gemma":[0.000019390356,0.000009732777,0.00021057519,0.0000015443048,0.0000026578712,0.0000052920022,0.000008746014,0.9990478,0.00018050401,0.00040189672,0.00011009119,0.0000016682081],"about_ca_topic_score_codex":0.009916501,"about_ca_topic_score_gemma":0.004719294,"teacher_disagreement_score":0.009916501,"about_ca_system_score_codex":0.0006211222,"about_ca_system_score_gemma":0.0005970542,"threshold_uncertainty_score":0.019717574},"labels":[],"label_agreement":null},{"id":"W2074992583","doi":"10.1088/0004-637x/763/2/82","title":"SPECTRAL AND TIMING PROPERTIES OF THE MAGNETAR CXOU J164710.2–455216","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Astrophysics; Black-body radiation; Physics; Flux (metallurgy); Neutron star; Photon; Materials science; Optics","score_opus":0.015762926015776658,"score_gpt":0.2616759374806778,"score_spread":0.24591301146490113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2074992583","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991142,0.00015048365,0.00009002103,0.000012069115,0.000004158622,0.0000030829071,0.00026227976,0.000010255925,0.00035342338],"genre_scores_gemma":[0.9979087,0.00009371693,0.00032669524,0.000013095541,0.000012477217,0.0000064490273,0.0012469247,0.000006285461,0.00038565169],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990594,0.0000057668326,0.000007477504,0.000031835283,0.000024698567,0.000024307281],"domain_scores_gemma":[0.99960524,0.000024139948,0.00022904023,0.000021815013,0.00004587887,0.000073918556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022466642,0.00026105464,0.0003297133,0.0009929584,0.00033829082,0.00035666567,0.00022580504,0.00030032158,0.0007085928],"category_scores_gemma":[0.00039646766,0.00013317165,0.00015187639,0.00052921055,0.00016986382,0.00017675644,0.00030089708,0.00018103242,0.00018182697],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038890145,0.000094568684,0.8072075,0.0001096722,0.000096983385,0.0011471007,0.0004933621,0.0013768773,0.16947372,0.00039706798,0.0006842809,0.018529955],"study_design_scores_gemma":[0.0000049604673,0.00007217077,0.99703634,0.0000053369,0.000012613619,0.00029359374,0.00004479181,0.000409071,0.0014218648,0.000024159106,0.00066668546,0.000008349322],"about_ca_topic_score_codex":0.004239352,"about_ca_topic_score_gemma":0.010870483,"teacher_disagreement_score":0.004239352,"about_ca_system_score_codex":0.00034707438,"about_ca_system_score_gemma":0.00010844014,"threshold_uncertainty_score":0.0084293485},"labels":[],"label_agreement":null},{"id":"W2075004811","doi":"10.1086/346234","title":"Radio Polarization from the Galactic Plane in Cygnus","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Faraday effect; Astrophysics; Polarization (electrochemistry); Galactic plane; Faraday cage; Linear polarization; Galaxy; Astronomy; Optics; Magnetic field","score_opus":0.007927778808640502,"score_gpt":0.20453393958803123,"score_spread":0.19660616077939072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075004811","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986242,0.00012054668,0.00012540384,0.000021638733,0.0000023681052,0.0000020190523,0.0001648437,0.000018112869,0.00092099165],"genre_scores_gemma":[0.99878067,0.00012686878,0.00021865276,0.000017410961,0.000015594838,0.0000046450327,0.00067925657,0.000006779941,0.00015017025],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999201,0.000010864825,0.0000021995038,0.000022066568,0.00002021122,0.000024519846],"domain_scores_gemma":[0.99983215,0.00002476703,0.000055771863,0.000012286952,0.00002492175,0.00005003808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110811765,0.00030309474,0.00020722687,0.0009964083,0.00024537908,0.00046628457,0.00016536209,0.00029065562,0.00051468844],"category_scores_gemma":[0.00034295226,0.00017088695,0.00011362689,0.0009800438,0.00026235636,0.00019367225,0.0004744297,0.000238231,0.0001885411],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080035225,0.00009978423,0.7711384,0.00013601998,0.00016753527,0.0015919685,0.0012390248,0.005008921,0.18194944,0.0009408949,0.0019495729,0.03497806],"study_design_scores_gemma":[0.000013843641,0.000030730218,0.9958682,0.000008637736,0.000021726495,0.00023610205,0.00006288245,0.0011553201,0.0016929765,0.00009849306,0.0008047353,0.0000063743237],"about_ca_topic_score_codex":0.008025907,"about_ca_topic_score_gemma":0.009431531,"teacher_disagreement_score":0.008025907,"about_ca_system_score_codex":0.00040609197,"about_ca_system_score_gemma":0.00015378278,"threshold_uncertainty_score":0.015958369},"labels":[],"label_agreement":null},{"id":"W2075098704","doi":"10.1086/518768","title":"Evidence of a Merger of Binary White Dwarfs: The Case of GD 362","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Astrophysics; Atmosphere (unit); Galaxy; Physics; Diffusion; Binary number; White (mutation); Astronomy; Chemistry; Stars; Meteorology","score_opus":0.021332312294430493,"score_gpt":0.2659208913044992,"score_spread":0.2445885790100687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075098704","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958812,0.00020889427,0.000082143146,0.00014608254,0.000011302209,0.0000057708917,0.0000634517,0.000008333361,0.0035928695],"genre_scores_gemma":[0.99951863,0.000064966815,0.00007754871,0.00004728817,0.000016361191,0.000001431759,0.00007750065,0.0000027460935,0.00019357775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999585,0.000040875064,0.00003667765,0.00011396124,0.00008414603,0.00013942357],"domain_scores_gemma":[0.99903584,0.00019943142,0.0002843568,0.00014012524,0.00009558399,0.00024465652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040355982,0.00052243844,0.0006326058,0.001233644,0.002239618,0.0019179628,0.00078296184,0.0021358267,0.0019135444],"category_scores_gemma":[0.0017149101,0.0003613776,0.0003857956,0.00095611846,0.0018245251,0.00075647817,0.0016192588,0.00059340324,0.00071876985],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021351064,0.0001304376,0.8486792,0.0001452051,0.00016409167,0.050689016,0.0031711308,0.00036837507,0.08192974,0.0055663786,0.0008129444,0.0062084435],"study_design_scores_gemma":[0.00025757434,0.00062021,0.84152406,0.000062074825,0.00028324506,0.11111158,0.006018059,0.00203864,0.020877281,0.003566879,0.013555983,0.00008441741],"about_ca_topic_score_codex":0.0068637617,"about_ca_topic_score_gemma":0.0044819694,"teacher_disagreement_score":0.0068637617,"about_ca_system_score_codex":0.00067878375,"about_ca_system_score_gemma":0.00030384527,"threshold_uncertainty_score":0.013647616},"labels":[],"label_agreement":null},{"id":"W2075106565","doi":"10.1088/0004-637x/795/1/45","title":"SYSTEMATIC UNCERTAINTIES ASSOCIATED WITH THE COSMOLOGICAL ANALYSIS OF THE FIRST PAN-STARRS1 TYPE Ia SUPERNOVA SAMPLE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":173,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; Queen's University; Johns Hopkins University; Queen's University Belfast; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"CMB cold spot; Physics; Astrophysics; Cosmic microwave background; Planck; Supernova; Redshift; Omega; Cosmic distance ladder; Galaxy; Flatness (cosmology); Systematic error; Calibration; Type (biology); Cosmology; Statistics","score_opus":0.011267892868523833,"score_gpt":0.22145525195680468,"score_spread":0.21018735908828085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075106565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97223324,0.0013512763,0.012224255,0.00019683749,0.000036948357,0.00003729231,0.004951683,0.0002988238,0.008669733],"genre_scores_gemma":[0.9895057,0.0002655608,0.0041355398,0.000042511776,0.000025225327,0.00002973058,0.00489016,0.00008739604,0.0010180534],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99582136,0.0013134797,0.00031205165,0.0011600856,0.0012324075,0.0001604643],"domain_scores_gemma":[0.98640037,0.0048361626,0.0025567845,0.004286769,0.001559175,0.00036064952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0055551357,0.0003648804,0.00043597788,0.0020195271,0.0004218364,0.00079140445,0.00066144305,0.00014705858,0.0015958726],"category_scores_gemma":[0.0135158375,0.00019663115,0.00065021886,0.0015786241,0.0003282774,0.00039246958,0.0014849465,0.00037307845,0.00052635465],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001157255,0.000031301104,0.93678784,0.00007725105,0.00038459274,0.00004655084,0.0003874868,0.003511301,0.0030236316,0.0022671472,0.001379305,0.05198782],"study_design_scores_gemma":[0.000005935707,0.000036797574,0.9870165,0.000033849057,0.00008209893,0.00012940992,0.0001030611,0.0038756796,0.0028512136,0.0011067798,0.0047415653,0.000017114582],"about_ca_topic_score_codex":0.006898793,"about_ca_topic_score_gemma":0.012992271,"teacher_disagreement_score":0.006898793,"about_ca_system_score_codex":0.00063623063,"about_ca_system_score_gemma":0.000405378,"threshold_uncertainty_score":0.029378712},"labels":[],"label_agreement":null},{"id":"W2075108887","doi":"10.1086/432753","title":"A Deep Infrared Search for AXP 1E 1841−045","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Pulsar; Photometry (optics); Infrared; Limiting; Limiting magnitude; Position (finance); Position angle; Near-infrared spectroscopy","score_opus":0.01792057499058535,"score_gpt":0.2602285061582953,"score_spread":0.24230793116770993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075108887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946461,0.0003243288,0.0008160176,0.00019710467,0.000012539236,0.000023259749,0.00025433302,0.00003695221,0.0036895112],"genre_scores_gemma":[0.99579334,0.00010766239,0.0017465409,0.00012284612,0.0000292112,0.000010202864,0.00096536294,0.000005331029,0.0012195443],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977213,0.00002115382,0.000011049946,0.00007093949,0.00007354455,0.000051204774],"domain_scores_gemma":[0.9994843,0.00007183337,0.00014978356,0.00004559845,0.000049050093,0.00019941365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005054274,0.0003258441,0.00029836412,0.0015411717,0.0008857036,0.0005603507,0.0003721721,0.00048470998,0.003330041],"category_scores_gemma":[0.00053122075,0.00023405682,0.0001795218,0.00075873476,0.00036883852,0.00044662543,0.00089723465,0.0004006779,0.000833488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006429878,0.00043363363,0.8256947,0.00017581836,0.00017946705,0.0032729595,0.0012060397,0.0003532021,0.08242418,0.0021435164,0.00342157,0.08005199],"study_design_scores_gemma":[0.00001695886,0.00028593198,0.99001956,0.000011232772,0.0000325469,0.0019957009,0.00023934594,0.0003457676,0.0019903225,0.0002993608,0.0047547813,0.000008447569],"about_ca_topic_score_codex":0.0007922771,"about_ca_topic_score_gemma":0.0019343173,"teacher_disagreement_score":0.003330041,"about_ca_system_score_codex":0.00027072348,"about_ca_system_score_gemma":0.00024162067,"threshold_uncertainty_score":0.011140108},"labels":[],"label_agreement":null},{"id":"W2075113123","doi":"10.1088/0004-637x/722/2/1864","title":"THE ACS LCID PROJECT. VI. THE STAR FORMATION HISTORY OF THE TUCANA dSph AND THE RELATIVE AGES OF THE ISOLATED dSph GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Local Group; Dwarf spheroidal galaxy; Star formation; Dwarf galaxy; Reionization; Astronomy; Milky Way; Stars; Lenticular galaxy","score_opus":0.007827081150779099,"score_gpt":0.20173502450340586,"score_spread":0.19390794335262676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075113123","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0020531814,0.00093153346,0.0032616614,0.0007447318,0.00027172765,0.00016997114,0.9314949,0.031028727,0.030043509],"genre_scores_gemma":[0.008059581,0.0007581716,0.016932543,0.00053146534,0.0001378918,0.0005872768,0.9543092,0.0067725303,0.011911261],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9989298,0.000064787695,0.000052787087,0.0002184153,0.0004883227,0.00024591354],"domain_scores_gemma":[0.99837154,0.00011771747,0.0001675477,0.00037295508,0.00058924814,0.00038097837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019098896,0.0021717574,0.0021419637,0.0052361214,0.0020465702,0.0064115385,0.0055931043,0.0015804899,0.12647629],"category_scores_gemma":[0.0030469915,0.0010608126,0.0012749692,0.008085917,0.00049631094,0.0025136434,0.0050946265,0.002172518,0.098380126],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028932682,0.00005490398,0.0027985454,0.00043072502,0.00012974403,0.00009822609,0.0001535582,0.00029139838,0.0009948608,0.0037699433,0.96535003,0.025638632],"study_design_scores_gemma":[0.00029031312,0.000014266931,0.007466941,0.00018103408,0.00011192813,0.00009723576,0.00011371612,0.0024315573,0.001590388,0.004579789,0.98305905,0.000063803986],"about_ca_topic_score_codex":0.12036618,"about_ca_topic_score_gemma":0.11294172,"teacher_disagreement_score":0.12647629,"about_ca_system_score_codex":0.0035218836,"about_ca_system_score_gemma":0.0046103797,"threshold_uncertainty_score":0.42310536},"labels":[],"label_agreement":null},{"id":"W2075158105","doi":"10.1086/381139","title":"Serendipity and the Sloan Digital Sky Survey: Discovery of the Largest Known Planetary Nebula on the Sky","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Sky; Planetary nebula; Physics; Nebula; White dwarf; Astrophysics; Astronomy; Emission nebula; Doubly ionized oxygen; Emission spectrum; Stars; Spectral line","score_opus":0.010035875177143418,"score_gpt":0.19921853411798154,"score_spread":0.18918265894083813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075158105","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98277587,0.0025400624,0.00024637047,0.000706526,0.000037349084,0.000010803127,0.003243273,0.000037152953,0.010402657],"genre_scores_gemma":[0.9898867,0.0017824816,0.00072803587,0.00011398088,0.00006079363,0.0000066250873,0.00488291,0.00000879067,0.0025296062],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992275,0.000007033438,0.000004200607,0.000015624155,0.000022927832,0.000027550604],"domain_scores_gemma":[0.99962187,0.000022626842,0.000119112396,0.000028280238,0.000060832368,0.00014727325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023210673,0.0001344063,0.000085236454,0.0014148254,0.00040243228,0.00053219986,0.00010955778,0.000113304806,0.0011165746],"category_scores_gemma":[0.00033933076,0.00007191181,0.000074078074,0.0010520612,0.0002458983,0.0002954722,0.0007135818,0.00020629105,0.00029951637],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010359494,0.000030820458,0.930488,0.00011146181,0.000041706797,0.0008315066,0.0006398416,0.00008124362,0.005676708,0.0010526207,0.0135338,0.047408696],"study_design_scores_gemma":[0.000002006959,0.0000072227617,0.986392,0.000009861544,0.000005920084,0.00026501136,0.00018534009,0.000029813637,0.00022615584,0.000058754562,0.012816334,0.0000016645084],"about_ca_topic_score_codex":0.018703222,"about_ca_topic_score_gemma":0.05616789,"teacher_disagreement_score":0.018703222,"about_ca_system_score_codex":0.0003435372,"about_ca_system_score_gemma":0.00038358037,"threshold_uncertainty_score":0.03718871},"labels":[],"label_agreement":null},{"id":"W2075241352","doi":"10.1088/0004-637x/735/1/13","title":"NEW CONSTRAINTS ON THE ORIGIN OF THE SHORT-TERM CYCLICAL VARIABILITY OF THE WOLF-RAYET STAR WR 46","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Astrophysics; Physics; Wolf–Rayet star; Light curve; Radial velocity; Context (archaeology); Spitzer Space Telescope; Astronomy; Telescope; Stars","score_opus":0.03070521094326954,"score_gpt":0.24401444746095488,"score_spread":0.21330923651768535,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075241352","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99601257,0.0006363752,0.00073637476,0.00008024178,0.000010721006,0.000005312686,0.00017375618,0.00003755201,0.0023071875],"genre_scores_gemma":[0.9990233,0.00015749775,0.00036166227,0.000022872784,0.000028454186,0.000004750979,0.00023799692,0.0000087481,0.00015470134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999192,0.000010070932,0.000010997824,0.000030284698,0.000013305337,0.000016195843],"domain_scores_gemma":[0.9991141,0.00018989925,0.0003548824,0.00014209673,0.00006847107,0.00013047665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034643902,0.00018826284,0.00029169166,0.00054617313,0.00028983128,0.0010192887,0.0003862541,0.000497069,0.0018760489],"category_scores_gemma":[0.0012525439,0.0001807985,0.00021431298,0.00059619383,0.00038683097,0.00075945194,0.0005443035,0.00042072177,0.00032730147],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046852537,0.00011263508,0.8013247,0.00015929085,0.0001292649,0.0013760695,0.0012483253,0.0020858129,0.14984131,0.0036893091,0.00065025315,0.038914397],"study_design_scores_gemma":[0.000009480841,0.000059196293,0.99033105,0.000021128075,0.000031121188,0.0005064928,0.00023223966,0.0028566227,0.0012516192,0.0017605772,0.0029226898,0.0000178015],"about_ca_topic_score_codex":0.0009344113,"about_ca_topic_score_gemma":0.0010459925,"teacher_disagreement_score":0.0018760489,"about_ca_system_score_codex":0.00024241072,"about_ca_system_score_gemma":0.00010222515,"threshold_uncertainty_score":0.0062760115},"labels":[],"label_agreement":null},{"id":"W2075246771","doi":"10.1088/0004-637x/697/2/1457","title":"THE INITIAL CONDITIONS OF CLUSTERED STAR FORMATION. I. NH<sub>3</sub>OBSERVATIONS OF DENSE CORES IN OPHIUCHUS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; James Clerk Maxwell Telescope; Interferometry; Telescope; Star formation; Submillimeter Array; Line (geometry); Green Bank Telescope; Giant Metrewave Radio Telescope","score_opus":0.02476926097446477,"score_gpt":0.2694321818086561,"score_spread":0.2446629208341913,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075246771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99846613,0.00010493743,0.00028382518,0.00002000336,0.0000018967042,0.000010821694,0.00015307877,0.000012601099,0.0009466945],"genre_scores_gemma":[0.9995264,0.000022451268,0.00020241381,0.0000066271086,0.0000019493682,0.0000036380734,0.00015277203,0.0000014406812,0.00008232799],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991894,0.000006278705,0.0000057200427,0.000018256751,0.000018893026,0.000031999058],"domain_scores_gemma":[0.9997019,0.00003273352,0.00009016207,0.00001520638,0.00005470187,0.00010525093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013943212,0.00015048143,0.0001571495,0.0003271215,0.0005385597,0.0005042021,0.00024114059,0.00031337704,0.0007956514],"category_scores_gemma":[0.0007794901,0.0001682318,0.00013319578,0.00017526363,0.00033182892,0.0002746544,0.00046869472,0.00029882014,0.00020313081],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028168136,0.00006750122,0.8731628,0.000076769094,0.00004283978,0.0008897782,0.0005428427,0.0041601057,0.11326442,0.0015530421,0.0005688948,0.0053893635],"study_design_scores_gemma":[0.000012796341,0.00007582322,0.98799765,0.000010470846,0.00000821414,0.00032009897,0.00043518658,0.0032115588,0.0066559706,0.00049658195,0.0007661936,0.00000951749],"about_ca_topic_score_codex":0.016077979,"about_ca_topic_score_gemma":0.019707793,"teacher_disagreement_score":0.016077979,"about_ca_system_score_codex":0.0010430326,"about_ca_system_score_gemma":0.00040027878,"threshold_uncertainty_score":0.031968772},"labels":[],"label_agreement":null},{"id":"W2075367943","doi":"10.1086/591219","title":"The Long‐Term Radiative Evolution of Anomalous X‐Ray Pulsar 1E 2259+586 After Its 2002 Outburst","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Research Canada; Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Physics; Pulsar; Astrophysics; Magnetar; Flux (metallurgy); Power law; Radiative transfer; Astronomy","score_opus":0.010792183379058296,"score_gpt":0.280981575088549,"score_spread":0.2701893917094907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075367943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996971,0.000021977836,0.00001710658,0.000009601415,0.0000012659995,9.06498e-7,0.000051674007,0.0000022934346,0.00019810315],"genre_scores_gemma":[0.99951386,0.00002685438,0.00004112799,0.000006175606,0.000005356502,0.0000016990384,0.00024557722,0.0000016255719,0.0001577522],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992824,0.0000074759027,0.0000062286117,0.000017881805,0.000018040264,0.000022147453],"domain_scores_gemma":[0.999405,0.00006996526,0.0002656105,0.00004538486,0.000110349225,0.000103796854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019793776,0.00018122066,0.0002559137,0.0006210361,0.0004101207,0.0005738039,0.00024315217,0.0002600364,0.00037881263],"category_scores_gemma":[0.0008792258,0.00010505324,0.00019508807,0.00040233927,0.0002080215,0.00024949978,0.00041923547,0.0002753282,0.00017578782],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023213807,0.00009531526,0.9743669,0.000018082854,0.000046091536,0.00066428643,0.00045477573,0.00051916565,0.015606876,0.00011870822,0.00018952845,0.007688193],"study_design_scores_gemma":[0.0000017426511,0.000033826578,0.9989537,0.0000019001203,0.000008637554,0.00017498505,0.00006740139,0.00023490716,0.00029967533,0.000015225606,0.00020526655,0.0000025879888],"about_ca_topic_score_codex":0.0051174616,"about_ca_topic_score_gemma":0.009108953,"teacher_disagreement_score":0.0051174616,"about_ca_system_score_codex":0.00031611035,"about_ca_system_score_gemma":0.000092928574,"threshold_uncertainty_score":0.010175407},"labels":[],"label_agreement":null},{"id":"W2075483162","doi":"10.1088/0004-637x/741/2/101","title":"SEARCH FOR<i>z</i>∼ 6.96 Lyα EMITTERS WITH MAGELLAN/IMACS IN THE COSMOS FIELD","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Luminosity; Luminosity function; Field (mathematics); Common emitter; Square (algebra); Sample (material); Cosmos (plant)","score_opus":0.022315476134265322,"score_gpt":0.2471124806897849,"score_spread":0.22479700455551957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075483162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99809617,0.00011628775,0.00022308613,0.00003127736,0.0000028124748,0.000012423798,0.0001502406,0.000018400622,0.0013492459],"genre_scores_gemma":[0.99733657,0.00010120446,0.0011470628,0.000044109016,0.000018552559,0.000009243204,0.0004923732,0.000010994763,0.00083996763],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997676,0.00001817185,0.000009886537,0.00006196482,0.00007178968,0.00007059525],"domain_scores_gemma":[0.9989064,0.00007696536,0.0004280313,0.00012096994,0.00013564345,0.00033195573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007937121,0.00033695166,0.00036661368,0.0015623755,0.0009242403,0.0007437695,0.00052688445,0.00029070023,0.002803176],"category_scores_gemma":[0.0006128215,0.00023315474,0.00026711202,0.0010622729,0.00022680624,0.00033835083,0.0004901521,0.00030241124,0.0011983127],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003822912,0.00013625826,0.9512861,0.00002750405,0.00005405933,0.00033824448,0.0002388378,0.000110770736,0.03538855,0.00023003135,0.00049964513,0.011307789],"study_design_scores_gemma":[0.000026848786,0.00021547954,0.9900247,0.000008724242,0.00004719313,0.0008980644,0.00017112224,0.00040029973,0.00566232,0.00013620239,0.0024016872,0.000007329654],"about_ca_topic_score_codex":0.0014926206,"about_ca_topic_score_gemma":0.002850628,"teacher_disagreement_score":0.002803176,"about_ca_system_score_codex":0.00022719103,"about_ca_system_score_gemma":0.00019873827,"threshold_uncertainty_score":0.009377539},"labels":[],"label_agreement":null},{"id":"W2075563071","doi":"10.1086/375490","title":"A Confirmation of the Optical Spectroscopy Approach: Discovery of Two More Pulsating DA (ZZ Ceti) White Dwarfs","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Instability strip; Physics; Astrophysics; Stars; Surface gravity; Spectroscopy; Light curve; Effective temperature; Luminosity; Spectral line; Homogeneous; Astronomy; Cepheid variable","score_opus":0.013965526247779358,"score_gpt":0.24457015910144494,"score_spread":0.2306046328536656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075563071","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9849231,0.0033078636,0.0047288816,0.0008672775,0.00008800051,0.000015910318,0.00013329464,0.000041548246,0.005894068],"genre_scores_gemma":[0.991089,0.0018354574,0.0048283366,0.0005044534,0.0002569426,0.000009102581,0.00019331745,0.000010234542,0.0012731234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998317,0.0000143943535,0.000018348257,0.00005898471,0.000055719527,0.00002086173],"domain_scores_gemma":[0.9992567,0.00018148567,0.00027231756,0.000060166716,0.0001353214,0.00009399687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005034054,0.00027485244,0.00013675647,0.0010512007,0.0003548488,0.00085910526,0.00030298697,0.0003731064,0.00034725227],"category_scores_gemma":[0.0009473257,0.00011517276,0.00016371928,0.00060689164,0.0005481946,0.00040525553,0.0005883849,0.00037610473,0.00014861186],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032289358,0.000079290476,0.73079616,0.00043846716,0.00009306676,0.002609827,0.0012021054,0.00081706647,0.14104721,0.008164769,0.00089878513,0.113530286],"study_design_scores_gemma":[0.000019565814,0.00038559572,0.9220972,0.00007667189,0.00010012152,0.0074838703,0.00063229736,0.001736088,0.037797406,0.0026244,0.027022863,0.000023931236],"about_ca_topic_score_codex":0.0012970243,"about_ca_topic_score_gemma":0.0012401975,"teacher_disagreement_score":0.0012970243,"about_ca_system_score_codex":0.00033258524,"about_ca_system_score_gemma":0.00020981506,"threshold_uncertainty_score":0.002662301},"labels":[],"label_agreement":null},{"id":"W2075626868","doi":"10.1088/0004-637x/772/1/35","title":"NUMERICAL ANALYSIS OF THE FOKKER-PLANCK EQUATION WITH ADIABATIC FOCUSING: ISOTROPIC PITCH-ANGLE SCATTERING","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Fokker–Planck equation; Adiabatic process; Isotropy; Numerical analysis; Diffusion; Distribution function; Numerical diffusion; Scattering; Classical mechanics; Pitch angle; Mathematical analysis; Statistical physics; Mechanics; Quantum mechanics; Mathematics; Differential equation","score_opus":0.007820810162353224,"score_gpt":0.2056356575044927,"score_spread":0.19781484734213947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075626868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5885586,0.0008958289,0.34895003,0.0024862525,0.00024524605,0.00017708719,0.0003965691,0.00045628834,0.057834208],"genre_scores_gemma":[0.92569494,0.00028363697,0.067887075,0.00018514751,0.000055701643,0.00016103301,0.00017920246,0.000087138964,0.0054660365],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997985,0.000042906653,0.000015614392,0.00002365895,0.00007933077,0.0000399733],"domain_scores_gemma":[0.99875927,0.00066835777,0.00016635265,0.00008902119,0.00024847675,0.0000685429],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068282883,0.00038732783,0.0005000684,0.0004908967,0.00074828183,0.0006320803,0.00093609013,0.001298118,0.00230131],"category_scores_gemma":[0.0036528353,0.00023576574,0.00044815624,0.0005954621,0.0011830961,0.0008300253,0.00075358764,0.00068778294,0.00017613881],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043963875,0.000036500933,0.0012061782,0.00006516497,0.000018995417,0.00016268178,0.00011418978,0.9528012,0.004411907,0.037575707,0.0004361802,0.0031272934],"study_design_scores_gemma":[0.000010567857,0.000004571958,0.00012287412,0.0000029210014,0.0000020104928,0.000013306573,0.000008835452,0.99777055,0.00038401425,0.0015154153,0.00016002242,0.000004978979],"about_ca_topic_score_codex":0.012065334,"about_ca_topic_score_gemma":0.0044891518,"teacher_disagreement_score":0.012065334,"about_ca_system_score_codex":0.0010737502,"about_ca_system_score_gemma":0.0011742102,"threshold_uncertainty_score":0.023990214},"labels":[],"label_agreement":null},{"id":"W2075733185","doi":"10.1086/386370","title":"The Contribution of Primordial Binaries to the Blue Straggler Population in 47 Tucanae","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Blue straggler; Astrophysics; Cluster (spacecraft); Globular cluster; Population; Core (optical fiber); Spatial distribution; Physics; Astronomy; Stars; Geography; Optics; Computer science; Demography","score_opus":0.006912754141863111,"score_gpt":0.22563835511916175,"score_spread":0.21872560097729865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075733185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996321,0.000047120706,0.00004007191,0.00000906584,8.0079525e-7,7.559237e-7,0.000041070532,0.0000040048585,0.00022500988],"genre_scores_gemma":[0.99962366,0.00004924518,0.00005213922,0.000004492914,0.0000010300141,9.828416e-7,0.000107205386,0.000003622705,0.00015752432],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998963,0.000006328578,0.000002310957,0.000023104447,0.000017221735,0.0000548712],"domain_scores_gemma":[0.9998031,0.000023001936,0.00003473808,0.000021151207,0.000037410104,0.00008063216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001564929,0.00016965857,0.00028959897,0.0010487995,0.0010803208,0.0010296749,0.0005176981,0.00037718727,0.0010979589],"category_scores_gemma":[0.0005887723,0.00015285212,0.00015492548,0.0007091901,0.0008002673,0.00026721187,0.00064973906,0.0002277202,0.00012143079],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004085319,0.00003128882,0.95993674,0.000019772813,0.0000528989,0.0003605216,0.0008856068,0.0032403932,0.02151381,0.0011617189,0.0002922883,0.012096496],"study_design_scores_gemma":[0.0000052756895,0.000022340155,0.99406475,0.0000026818761,0.000018841045,0.00014539964,0.0005002083,0.003297517,0.0011883697,0.0002535926,0.0004887235,0.000012305398],"about_ca_topic_score_codex":0.19024906,"about_ca_topic_score_gemma":0.15848805,"teacher_disagreement_score":0.19024906,"about_ca_system_score_codex":0.0020502168,"about_ca_system_score_gemma":0.000658186,"threshold_uncertainty_score":0.37828338},"labels":[],"label_agreement":null},{"id":"W2075832659","doi":"10.1086/511849","title":"The Bound Mass of Substructures in Dark Matter Halos","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Halo; Physics; Astrophysics; Dark matter; Cluster (spacecraft); Substructure; Galaxy","score_opus":0.004738435027590971,"score_gpt":0.21144087594016805,"score_spread":0.20670244091257708,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075832659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97608656,0.00022528236,0.021653535,0.000057389694,0.0000045381994,0.00000998811,0.00015686305,0.00008200633,0.001723858],"genre_scores_gemma":[0.9943135,0.00008371224,0.005147363,0.000018441317,0.000005540854,0.000010156929,0.00014460924,0.00003868101,0.00023799937],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982303,0.00003878751,0.000010210064,0.000052958785,0.00005044205,0.000024552306],"domain_scores_gemma":[0.9993437,0.00017210486,0.00016866214,0.00014123975,0.00003769503,0.0001366218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004994855,0.00031064812,0.00035276063,0.001117642,0.00043830747,0.0014441129,0.00071619893,0.000360972,0.000795504],"category_scores_gemma":[0.0029175954,0.00025758095,0.0003355137,0.0006808197,0.000932115,0.00093794795,0.0016273189,0.00036495953,0.00014105838],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032222352,0.000085073996,0.28980294,0.000105500745,0.00024302342,0.00035644879,0.0015369832,0.61405563,0.024770327,0.048147466,0.0006440376,0.01993041],"study_design_scores_gemma":[0.000040290335,0.000039564136,0.111874565,0.00003639109,0.000050585357,0.00011138659,0.0002455503,0.8532394,0.0071303356,0.024981542,0.0021999853,0.00005037113],"about_ca_topic_score_codex":0.004203475,"about_ca_topic_score_gemma":0.0040987455,"teacher_disagreement_score":0.004203475,"about_ca_system_score_codex":0.0006400397,"about_ca_system_score_gemma":0.0002269131,"threshold_uncertainty_score":0.008358002},"labels":[],"label_agreement":null},{"id":"W2075833520","doi":"10.1086/308832","title":"Large‐Scale QSO‐Galaxy Correlations and Weak Lensing","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"QSOS; Weak gravitational lensing; Redshift; Galaxy; Strong gravitational lensing; Cosmology; Amplitude; Gravitational lens; Gravitational lensing formalism","score_opus":0.005852830240256732,"score_gpt":0.20366667015153767,"score_spread":0.19781383991128093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075833520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98541,0.0002629687,0.011235208,0.00022889908,0.000007664823,0.00000770212,0.00004971333,0.000057697685,0.0027402623],"genre_scores_gemma":[0.99934584,0.00007588684,0.00040950158,0.000009169431,0.0000061327423,0.0000016020446,0.00001278733,0.0000033472463,0.00013570854],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99981886,0.000065481036,0.000011837701,0.000027674136,0.000047018664,0.000029281942],"domain_scores_gemma":[0.99716944,0.0014203787,0.00091574754,0.0001951149,0.00014256706,0.00015677951],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006550543,0.00027521246,0.00023500201,0.00035565367,0.00023104515,0.00076529995,0.0003206356,0.00019378381,0.0014792919],"category_scores_gemma":[0.005471272,0.00023090397,0.00016839115,0.00039210997,0.0010732608,0.0007231761,0.0005226319,0.00032367095,0.000084540625],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032110544,0.00010417139,0.30551484,0.00026578884,0.00024087238,0.001372418,0.00056090107,0.3145868,0.035990626,0.3134371,0.0019317474,0.025673581],"study_design_scores_gemma":[0.00006989036,0.00006502518,0.19609608,0.000019085945,0.000058938334,0.00028439614,0.00016308352,0.6804477,0.009188803,0.112484515,0.001071107,0.000051412077],"about_ca_topic_score_codex":0.004631083,"about_ca_topic_score_gemma":0.0032365585,"teacher_disagreement_score":0.004631083,"about_ca_system_score_codex":0.0006444894,"about_ca_system_score_gemma":0.00027459496,"threshold_uncertainty_score":0.009208262},"labels":[],"label_agreement":null},{"id":"W2075879481","doi":"10.1086/513175","title":"Saving Planetary Systems: Dead Zones and Planetary Migration","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McMaster University","funders":"","keywords":"Planet; Planetary migration; Dead zone; Physics; RADIUS; Planetary mass; Astrophysics; Geology; Planetary system; Computer science","score_opus":0.009122743888000003,"score_gpt":0.21819993275651106,"score_spread":0.20907718886851107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2075879481","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94238836,0.0007090508,0.04347955,0.00076025445,0.00009283486,0.00003650293,0.00016230976,0.00031549152,0.0120557025],"genre_scores_gemma":[0.9915174,0.00019238704,0.006484054,0.00004294746,0.0000068315912,0.000022563188,0.000045538534,0.000041449905,0.0016467542],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998919,0.000039135528,0.0000045978745,0.000016395828,0.000027300346,0.000020620475],"domain_scores_gemma":[0.99951077,0.00021909532,0.00008249584,0.00005415418,0.00004099003,0.00009257459],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026432655,0.00036676714,0.00039737596,0.000278228,0.00073633273,0.000971528,0.000745398,0.0009005312,0.0032105958],"category_scores_gemma":[0.0025127826,0.00024709362,0.00026549798,0.00031190968,0.0013855314,0.0017337309,0.001300387,0.0007776509,0.00022989546],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001247387,0.000059259834,0.0092737675,0.00011097051,0.00003694055,0.00025162564,0.0006661266,0.9333807,0.004310953,0.041591924,0.0008996111,0.009293352],"study_design_scores_gemma":[0.000055513123,0.00007019176,0.002065742,0.000019535504,0.000010731784,0.00008314923,0.00026043315,0.97602683,0.0011520723,0.017409103,0.0028260872,0.000020663145],"about_ca_topic_score_codex":0.0058778524,"about_ca_topic_score_gemma":0.003409156,"teacher_disagreement_score":0.0058778524,"about_ca_system_score_codex":0.0005174685,"about_ca_system_score_gemma":0.00047326114,"threshold_uncertainty_score":0.011687279},"labels":[],"label_agreement":null},{"id":"W2076056673","doi":"10.1086/444347","title":"Fireballs from Quark Stars in the Color‐Flavor Locked Phase: Application to Gamma‐Ray Bursts","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Quark star; Strange matter; Astrophysics; Stars; Gamma-ray burst; Accretion (finance); Color superconductivity; Millisecond; Quark; Strange quark; Phase (matter); Astronomy; Particle physics","score_opus":0.008842586249739683,"score_gpt":0.2576054210100974,"score_spread":0.24876283476035774,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076056673","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9830116,0.001651488,0.012044728,0.00009198921,0.00003833299,0.000041903393,0.000047119993,0.00010722891,0.0029656251],"genre_scores_gemma":[0.9963243,0.00076572475,0.0024080528,0.000024840258,0.000017916831,0.000010723093,0.000037511534,0.00000671723,0.0004041739],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992204,0.000017584347,0.000006669531,0.000016969101,0.000015302101,0.000021488404],"domain_scores_gemma":[0.9996253,0.00012842921,0.000082369916,0.000053404325,0.00003837643,0.00007206748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031203308,0.00032401268,0.00039068787,0.000511947,0.0005532272,0.0013386626,0.00034560327,0.0005800655,0.00077537],"category_scores_gemma":[0.00083189114,0.00019922775,0.00035931708,0.00041175997,0.0005920234,0.00037919168,0.00067966606,0.00030766096,0.000105093925],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014965789,0.0003242747,0.16728787,0.00041620046,0.00013197272,0.009000324,0.0009344162,0.019074792,0.65470827,0.06226131,0.00058156106,0.083782524],"study_design_scores_gemma":[0.0005565769,0.0015808532,0.21361588,0.00015060941,0.00029444572,0.022579027,0.0009817164,0.3560216,0.30696294,0.08735472,0.009739163,0.0001624306],"about_ca_topic_score_codex":0.0010807259,"about_ca_topic_score_gemma":0.00055576063,"teacher_disagreement_score":0.0013386626,"about_ca_system_score_codex":0.00037971238,"about_ca_system_score_gemma":0.00014410245,"threshold_uncertainty_score":0.0027549863},"labels":[],"label_agreement":null},{"id":"W2076107312","doi":"10.1086/498144","title":"Starburst Models for Far‐Infrared/Submillimeter/Millimeter Line Emission. I. An Expanding Supershell Surrounding a Massive Star Cluster","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Millimeter; Submillimeter Array; Interstellar medium; Supernova; Star formation; Molecular cloud; Far infrared; Infrared; Cluster (spacecraft); Galaxy; Shell (structure); Line (geometry); Astronomy; Cosmic dust; Materials science; Stars","score_opus":0.022663622398106955,"score_gpt":0.26109142552212256,"score_spread":0.2384278031240156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076107312","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.76290035,0.0015328815,0.18440893,0.0014033174,0.00016899535,0.00012761865,0.0013469907,0.0007085947,0.047402337],"genre_scores_gemma":[0.9751898,0.0006075254,0.009759627,0.00012442595,0.00007198625,0.00011770561,0.0004686994,0.00009575086,0.013564589],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990106,0.000026263768,0.000004520252,0.000024484516,0.000017564485,0.000026169584],"domain_scores_gemma":[0.99972016,0.00007305944,0.00008311716,0.00002195423,0.00003470791,0.000067107525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002955736,0.00057125144,0.00036780495,0.00030343764,0.00053978385,0.0011318517,0.0014880367,0.00082971534,0.0040282975],"category_scores_gemma":[0.000716014,0.0003083757,0.00061861373,0.00033353627,0.000618304,0.0009605844,0.000798111,0.00053748745,0.0008244016],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013019526,0.000072431896,0.015812911,0.00008479032,0.00008890747,0.0007763286,0.0004466679,0.87873864,0.0058330833,0.09121993,0.0020966553,0.0046995045],"study_design_scores_gemma":[0.0000408035,0.00003461185,0.004028116,0.000011482405,0.000027862108,0.000164324,0.000097110875,0.97690237,0.00022804207,0.016116066,0.0023384346,0.00001078086],"about_ca_topic_score_codex":0.018900605,"about_ca_topic_score_gemma":0.01134479,"teacher_disagreement_score":0.018900605,"about_ca_system_score_codex":0.0011241458,"about_ca_system_score_gemma":0.00044073712,"threshold_uncertainty_score":0.037581205},"labels":[],"label_agreement":null},{"id":"W2076134248","doi":"10.1088/0004-637x/755/1/15","title":"MODELS FOR METAL-POOR STARS WITH ENHANCED ABUNDANCES OF C, N, O, Ne, Na, Mg, Si, S, Ca, AND Ti, IN TURN, AT CONSTANT HELIUM AND IRON ABUNDANCES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":143,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Regina; Université de Montréal; University of Victoria","funders":"","keywords":"Astrophysics; Physics; Helium; Stars; Abundance (ecology); Metal; Abundance of the chemical elements; Globular cluster; Oxygen; Luminosity; Analytical Chemistry (journal); Cluster (spacecraft); Chemistry; Materials science; Atomic physics; Galaxy; Metallurgy","score_opus":0.01095106788494674,"score_gpt":0.2235532174883609,"score_spread":0.21260214960341417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076134248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8612725,0.00051491224,0.10514312,0.0009973327,0.0000972152,0.00020077212,0.0021153248,0.0007429905,0.028915863],"genre_scores_gemma":[0.94442385,0.00036939094,0.020751515,0.0001774209,0.000050607407,0.00031106875,0.001449426,0.00020565056,0.032260943],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983764,0.00004390531,0.0000073731508,0.000041246483,0.000025753117,0.000044039418],"domain_scores_gemma":[0.99963033,0.000104068975,0.00005739024,0.000028067328,0.00007878864,0.000101337435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057446194,0.00074249046,0.0006920007,0.00076520257,0.0008629836,0.0013910307,0.0029640996,0.0013642391,0.004235061],"category_scores_gemma":[0.000917981,0.0005742356,0.0011850547,0.0006660482,0.0005865971,0.001291345,0.0008314549,0.0007292156,0.0011464707],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018569773,0.000075976015,0.012120024,0.000046218753,0.00007844101,0.00019209206,0.00018355582,0.9627656,0.0023827238,0.018487547,0.001107364,0.002374903],"study_design_scores_gemma":[0.00008805326,0.00003911836,0.0030651225,0.000009700181,0.00003319214,0.000074259384,0.00008344176,0.98173964,0.00030918283,0.012466957,0.0020671452,0.000024284973],"about_ca_topic_score_codex":0.025467306,"about_ca_topic_score_gemma":0.031293835,"teacher_disagreement_score":0.025467306,"about_ca_system_score_codex":0.0022159133,"about_ca_system_score_gemma":0.0009315938,"threshold_uncertainty_score":0.05063814},"labels":[],"label_agreement":null},{"id":"W2076295538","doi":"10.1088/0004-637x/771/2/137","title":"<i>WMAP</i>OBSERVATIONS OF<i>PLANCK</i>ESZ CLUSTERS","year":2013,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of British Columbia","funders":"","keywords":"CMB cold spot; Amplitude; Planck; Cosmic microwave background; Cosmic background radiation; Cosmology","score_opus":0.012261183551345695,"score_gpt":0.2322791503210754,"score_spread":0.2200179667697297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076295538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99073994,0.000111530055,0.00082866766,0.00012779694,0.000008854527,0.00000582415,0.005095647,0.00009523245,0.002986544],"genre_scores_gemma":[0.98847264,0.00012815032,0.0018481491,0.00006176153,0.000036536912,0.000020320462,0.0086633805,0.000057505742,0.00071158714],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978584,0.000026297908,0.000013565357,0.000060090457,0.000058915448,0.000055379205],"domain_scores_gemma":[0.99894327,0.00015477806,0.00043655557,0.00022694084,0.0001237417,0.00011473491],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006212984,0.00033138352,0.00024866668,0.0018756419,0.00033331182,0.00077835924,0.00034684516,0.00024158704,0.0016040464],"category_scores_gemma":[0.0012441593,0.00026421895,0.00039441165,0.0025610207,0.00025706182,0.00034188677,0.0008261041,0.0003385657,0.0005409518],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002904273,0.000065936176,0.91419446,0.00011703175,0.0008477607,0.0003197515,0.0010147505,0.011532833,0.023557492,0.0062186997,0.015555225,0.026285714],"study_design_scores_gemma":[0.0000049273185,0.000007048264,0.9924838,0.000005771408,0.000039004568,0.000028911938,0.000099205114,0.0013023419,0.0024798762,0.00032585044,0.0032095853,0.000013730492],"about_ca_topic_score_codex":0.010555677,"about_ca_topic_score_gemma":0.010259253,"teacher_disagreement_score":0.010555677,"about_ca_system_score_codex":0.00035766963,"about_ca_system_score_gemma":0.00023393589,"threshold_uncertainty_score":0.020988464},"labels":[],"label_agreement":null},{"id":"W2076356472","doi":"10.1088/0004-637x/800/2/93","title":"WIDE FIELD MULTIBAND IMAGING OF LOW REDSHIFT QUASAR ENVIRONMENTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Quasar; Sky; Redshift; Astronomy; Radio galaxy; Amplitude; Observatory; Telescope","score_opus":0.007804006067154393,"score_gpt":0.2122548632264356,"score_spread":0.2044508571592812,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076356472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971264,0.00008334845,0.0013270283,0.000019448145,0.0000027288668,0.000003632967,0.00033972276,0.00005702597,0.0010406369],"genre_scores_gemma":[0.9972276,0.000057727422,0.0016839196,0.000025121117,0.000011223977,0.000005531971,0.0005182844,0.00001082299,0.00045977443],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999132,0.0000059953427,0.000003296456,0.000031318286,0.000017822735,0.000028254239],"domain_scores_gemma":[0.9997217,0.000037860274,0.00007617661,0.000033686152,0.0000396258,0.00009098489],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001724689,0.00014379129,0.00012732124,0.0010936206,0.00017224556,0.00031854055,0.0002032271,0.00017835376,0.0011245989],"category_scores_gemma":[0.0002461218,0.00014172817,0.00013296684,0.00044175732,0.000115109295,0.00025017577,0.0003066001,0.0001716041,0.0002551307],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003974783,0.00019739896,0.45063332,0.00007237326,0.00011389258,0.00045071513,0.00042154104,0.0024172901,0.4997694,0.00056046044,0.0013532536,0.04361292],"study_design_scores_gemma":[0.000004352634,0.000048789167,0.9937816,0.0000033996025,0.000014714062,0.0002418234,0.00006453832,0.0011820347,0.004059279,0.000088712775,0.0005048687,0.0000057324514],"about_ca_topic_score_codex":0.0015278136,"about_ca_topic_score_gemma":0.005272006,"teacher_disagreement_score":0.0015278136,"about_ca_system_score_codex":0.00014804796,"about_ca_system_score_gemma":0.00006169495,"threshold_uncertainty_score":0.003762126},"labels":[],"label_agreement":null},{"id":"W2076359355","doi":"10.1086/524887","title":"Ram Pressure Stripping of an Isolated Local Group Dwarf Galaxy: Evidence for an Intragroup Medium","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Dwarf galaxy; Astrophysics; Ram pressure; Local Group; Galaxy; Physics; Galaxy group; Stripping (fiber); Group (periodic table); Stars; Astronomy; Galaxy formation and evolution; Star formation; Materials science","score_opus":0.016774388429153523,"score_gpt":0.2623457850127887,"score_spread":0.2455713965836352,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076359355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990977,0.00007802849,0.0000820676,0.0000076411525,7.610132e-7,0.0000012225307,0.000017802933,0.0000073504293,0.00070750446],"genre_scores_gemma":[0.99980634,0.000023753413,0.00006080809,0.0000045739353,0.0000021855583,5.8965105e-7,0.000024888044,0.0000013076093,0.00007553759],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999459,0.0000037691443,0.0000019242516,0.000015772734,0.000011847426,0.000020885493],"domain_scores_gemma":[0.9997695,0.000032461532,0.00007696776,0.000030430352,0.000013184066,0.00007735866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006739645,0.0002123639,0.00028181152,0.00067102676,0.00035867796,0.0005166287,0.0003393419,0.00021914055,0.0011842207],"category_scores_gemma":[0.00021811828,0.00010512619,0.0001055977,0.00038532016,0.00040995458,0.00031816997,0.0008154172,0.00016750461,0.00021843442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011567117,0.00018137498,0.49575195,0.0001512511,0.00018779642,0.005788668,0.0020966476,0.00083058485,0.46199587,0.00096458296,0.00029239082,0.030602165],"study_design_scores_gemma":[0.000030494351,0.00024738628,0.9708774,0.000011496573,0.000092550086,0.002310523,0.0008991966,0.0018243305,0.02200456,0.0004226265,0.0012667972,0.000012711621],"about_ca_topic_score_codex":0.0017866481,"about_ca_topic_score_gemma":0.002073863,"teacher_disagreement_score":0.0017866481,"about_ca_system_score_codex":0.00020321488,"about_ca_system_score_gemma":0.000056043,"threshold_uncertainty_score":0.0039616227},"labels":[],"label_agreement":null},{"id":"W2076392377","doi":"10.1086/427183","title":"The DEEP2 Galaxy Redshift Survey: Evolution of Close Galaxy Pairs and Major-Merger Rates up to <i>z</i> ~ 1.2","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":267,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University","funders":"","keywords":"Astrophysics; Physics; Redshift; Galaxy; Redshift survey; Luminosity; Galaxy formation and evolution; Galaxy merger; Astronomy","score_opus":0.007309717372281625,"score_gpt":0.21992475937697284,"score_spread":0.21261504200469122,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076392377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936227,0.00034797232,0.00030583199,0.000063268206,0.000003348778,0.0000050570006,0.0038265116,0.000025780631,0.0017996144],"genre_scores_gemma":[0.99401724,0.0001784546,0.0003452309,0.000022845368,0.0000061724013,0.00000528744,0.0047934973,0.0000070873098,0.00062421197],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998667,0.000021703212,0.0000075709,0.000037592454,0.000024820498,0.000041509273],"domain_scores_gemma":[0.99871206,0.00013684113,0.00052205543,0.00011541854,0.00017620067,0.00033745734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043403264,0.00032100902,0.00020698062,0.0020436486,0.00028836136,0.00057994766,0.00031880854,0.00032508388,0.0014365133],"category_scores_gemma":[0.0010462586,0.00023056894,0.00032713206,0.001669704,0.00020437708,0.000621482,0.00095674454,0.00031266766,0.0005484199],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010409028,0.000023968107,0.99159735,0.000028116561,0.000059859474,0.00007489195,0.00018475014,0.00046162197,0.0014050085,0.0003579921,0.0007268333,0.004975528],"study_design_scores_gemma":[0.0000032985863,0.000014191718,0.9984547,0.0000030336341,0.000011617536,0.00009140933,0.00004322539,0.0003183979,0.00020300479,0.00005782575,0.0007963798,0.0000029469186],"about_ca_topic_score_codex":0.017325325,"about_ca_topic_score_gemma":0.024657343,"teacher_disagreement_score":0.017325325,"about_ca_system_score_codex":0.0004929354,"about_ca_system_score_gemma":0.00018212436,"threshold_uncertainty_score":0.03444892},"labels":[],"label_agreement":null},{"id":"W2076406066","doi":"10.1086/589506","title":"Discovery of the Radio and X-Ray Counterpart of TeV γ-Ray Source HESS J1731-347","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"X-ray; Physics; Astrophysics; Astronomy; Nuclear physics","score_opus":0.006599134430809327,"score_gpt":0.1947944704014483,"score_spread":0.18819533597063895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076406066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978479,0.000101604586,0.00024255435,0.000033374563,0.000009087851,0.000006312061,0.00023895678,0.000034112367,0.0014861218],"genre_scores_gemma":[0.9976841,0.000068575566,0.00063708617,0.0000414683,0.000016698032,0.000005112062,0.0009710986,0.000013420996,0.0005624872],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993956,0.0000026348334,0.000002883748,0.000020607735,0.000016854516,0.00001747672],"domain_scores_gemma":[0.9997689,0.0000138393,0.00005961011,0.000027898146,0.000022365157,0.00010736156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009475699,0.00018596013,0.00020771232,0.0006527764,0.00029200886,0.0004696406,0.00031760024,0.00027342225,0.0012632242],"category_scores_gemma":[0.00020605985,0.00010773412,0.00018386486,0.00049174647,0.00026123913,0.00016994028,0.0006307488,0.00022626841,0.0005245726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005384942,0.00010409482,0.80006003,0.00011590963,0.0001418606,0.013354815,0.00088166544,0.0010510277,0.15501873,0.0024032225,0.0026042252,0.023725897],"study_design_scores_gemma":[0.000035550776,0.00018930755,0.97771704,0.000019158026,0.000057395722,0.004864923,0.00032401763,0.001476471,0.0060110493,0.0005993927,0.008675575,0.00003005731],"about_ca_topic_score_codex":0.002107994,"about_ca_topic_score_gemma":0.0035515858,"teacher_disagreement_score":0.002107994,"about_ca_system_score_codex":0.00024477433,"about_ca_system_score_gemma":0.00017474683,"threshold_uncertainty_score":0.0042259097},"labels":[],"label_agreement":null},{"id":"W2076407791","doi":"10.1086/343795","title":"Model Atmosphere Analysis of Two Very Cool White Dwarfs","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Atmosphere (unit); Stars; Context (archaeology); Stellar atmosphere; Hydrogen; Infrared; Energy distribution","score_opus":0.016442110541492777,"score_gpt":0.22915491559614512,"score_spread":0.21271280505465234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076407791","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9702167,0.00014897018,0.016029932,0.00016665693,0.000017369493,0.00003020348,0.0021181547,0.0006897686,0.010582242],"genre_scores_gemma":[0.9910405,0.000108719374,0.004955627,0.00003242665,0.000010781381,0.000038203198,0.0016566551,0.00018906446,0.0019681533],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999131,0.000023833714,0.0000037250427,0.000019204863,0.00002137975,0.000018858605],"domain_scores_gemma":[0.99982965,0.00006261918,0.000016803619,0.000022827544,0.00003670738,0.000031394313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017137371,0.0004135593,0.00042935024,0.00038652887,0.0005203268,0.00062966946,0.00058110495,0.00037602746,0.0015354063],"category_scores_gemma":[0.00063759217,0.00019433987,0.0006139881,0.00031425574,0.00017703726,0.0002679461,0.00046484714,0.00035694955,0.00027389528],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012321453,0.000057520225,0.028192958,0.00003545912,0.000098116834,0.00026405207,0.00016985337,0.95047975,0.0060969586,0.0085785715,0.0012062605,0.004697195],"study_design_scores_gemma":[0.00006307137,0.000030516663,0.010541089,0.0000027649248,0.00003642404,0.00004830747,0.00005367842,0.9831708,0.0009006315,0.0028461306,0.0022896677,0.00001695438],"about_ca_topic_score_codex":0.026266184,"about_ca_topic_score_gemma":0.014867497,"teacher_disagreement_score":0.026266184,"about_ca_system_score_codex":0.0008360489,"about_ca_system_score_gemma":0.00049154565,"threshold_uncertainty_score":0.052226603},"labels":[],"label_agreement":null},{"id":"W2076474198","doi":"10.1088/0004-637x/757/2/169","title":"THE X-RAY TRANSIENT 2XMMi J003833.3+402133: A CANDIDATE MAGNETAR AT HIGH GALACTIC LATITUDE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Magnetar; Physics; Astrophysics; ROSAT; Pulsar; Neutron star; Astronomy; Milky Way; Black-body radiation; Supernova; Galactic plane; Black hole (networking); Galaxy; RADIUS; Luminosity; Telescope; Light curve; Radiation","score_opus":0.009363828903182655,"score_gpt":0.21779796391951875,"score_spread":0.2084341350163361,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076474198","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985337,0.00012189927,0.00013198504,0.000057367153,0.0000031187556,0.0000055235655,0.00011163566,0.000023114366,0.0010115624],"genre_scores_gemma":[0.99875927,0.00007210014,0.00030626738,0.000038636914,0.000012272808,0.0000052467904,0.00035875847,0.0000067045166,0.00044073787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999305,0.0000041776557,0.000002869569,0.000017793676,0.0000114774775,0.000033248416],"domain_scores_gemma":[0.9997781,0.00001385267,0.00011490474,0.000013828846,0.000014283599,0.00006502385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000114133814,0.00031165106,0.00032465678,0.00057383534,0.0006360354,0.00061135745,0.00043665897,0.00056346477,0.0014701785],"category_scores_gemma":[0.00020277145,0.00018067786,0.0002057318,0.0007184997,0.00024877102,0.00028678845,0.0004803105,0.00026418394,0.0005861441],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004648551,0.00012475316,0.8737928,0.00011062978,0.00005337451,0.013833764,0.0008379794,0.0007012228,0.09752902,0.0008677227,0.0013881392,0.010295643],"study_design_scores_gemma":[0.000011196943,0.00010329082,0.98902506,0.000013004721,0.000029904797,0.0040284963,0.000393777,0.00089613494,0.0027056402,0.00019640841,0.002584785,0.000012277679],"about_ca_topic_score_codex":0.0026143268,"about_ca_topic_score_gemma":0.007117913,"teacher_disagreement_score":0.0026143268,"about_ca_system_score_codex":0.0004918376,"about_ca_system_score_gemma":0.00020067095,"threshold_uncertainty_score":0.0051981807},"labels":[],"label_agreement":null},{"id":"W2076505864","doi":"10.1086/320437","title":"The Trajectory of the Jet in NGC 4258","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Jet (fluid); Galaxy; Thick disk; RADIUS; Ram pressure; Plane (geometry); Spiral galaxy; Thin disk; Amplitude; Astronomy; Disc; Halo; Galaxy formation and evolution; Mechanics; Geometry; Star formation; Optics","score_opus":0.007476017968547684,"score_gpt":0.21268485195749462,"score_spread":0.20520883398894693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076505864","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970392,0.00006956559,0.00022548602,0.000025421958,0.0000028370102,0.0000021360356,0.00009664398,0.000028753688,0.0025100217],"genre_scores_gemma":[0.9992932,0.00003167107,0.00022454758,0.0000040089913,9.898082e-7,9.2866276e-7,0.000101023485,0.0000039599086,0.00033967115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999733,0.000003883889,0.0000014574505,0.00000829529,0.0000068837967,0.0000062107947],"domain_scores_gemma":[0.9999126,0.000015279995,0.00002595227,0.000009337232,0.000013604729,0.00002315558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004921176,0.000109192224,0.00007646372,0.0003183399,0.00026772442,0.0004959227,0.00016392938,0.00024299596,0.0010434267],"category_scores_gemma":[0.00033747425,0.00009599763,0.00010470331,0.00026706056,0.00018246472,0.00015325243,0.00021407627,0.00015789089,0.0001656365],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047293262,0.00011646151,0.73333645,0.000112360365,0.000117904914,0.004994466,0.0023440628,0.07190838,0.13575928,0.013208888,0.002276257,0.035352483],"study_design_scores_gemma":[0.00004952215,0.00016234188,0.91571283,0.000040400304,0.000042622538,0.0004839352,0.0007620191,0.071356036,0.003951701,0.0025223466,0.0048744204,0.00004181138],"about_ca_topic_score_codex":0.030719792,"about_ca_topic_score_gemma":0.032076478,"teacher_disagreement_score":0.030719792,"about_ca_system_score_codex":0.0007382579,"about_ca_system_score_gemma":0.00017305897,"threshold_uncertainty_score":0.061081946},"labels":[],"label_agreement":null},{"id":"W2076561139","doi":"10.1088/0004-637x/734/1/25","title":"ARE PROTO-PLANETARY NEBULAE SHAPED BY A BINARY? RESULTS OF A LONG-TERM RADIAL VELOCITY STUDY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Planetary nebula; Binary number; Radial velocity; Binary star; Nebula; Stellar classification; Orbital elements; Limiting; Stellar evolution","score_opus":0.025416579407533765,"score_gpt":0.23918911528283773,"score_spread":0.21377253587530398,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076561139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99501956,0.0014022022,0.00047343198,0.00004590157,0.0000074165773,0.000003875995,0.00010869549,0.00000632464,0.0029325078],"genre_scores_gemma":[0.9986285,0.00031620482,0.0002823814,0.000026750675,0.0000123295495,0.000003078533,0.00026310197,0.000004704644,0.00046297102],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996458,0.00005920242,0.000038048656,0.000101357655,0.000086077096,0.00006957041],"domain_scores_gemma":[0.99838364,0.00043329064,0.00043625064,0.0002925292,0.00026720064,0.00018713872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007546426,0.0001171469,0.00031981157,0.0006689162,0.00055346347,0.00087874837,0.00027487078,0.00031698946,0.0015854473],"category_scores_gemma":[0.0023578024,0.00010473676,0.00023266308,0.00067081995,0.0005786085,0.0006820988,0.00040639137,0.00026732092,0.000833735],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003337248,0.00008642511,0.9602055,0.000052900792,0.00005822396,0.00065245404,0.0006243478,0.00016370538,0.014503571,0.00069371617,0.0001628558,0.022462616],"study_design_scores_gemma":[0.0000041175754,0.0001065027,0.99235016,0.00001737571,0.000042576365,0.0023131853,0.0004490423,0.00022018766,0.0018105148,0.00050276803,0.0021767968,0.0000067920632],"about_ca_topic_score_codex":0.001288329,"about_ca_topic_score_gemma":0.0010963833,"teacher_disagreement_score":0.0015854473,"about_ca_system_score_codex":0.00027317315,"about_ca_system_score_gemma":0.00014690567,"threshold_uncertainty_score":0.0053038597},"labels":[],"label_agreement":null},{"id":"W2076572859","doi":"10.1086/378583","title":"Evidence for Planet‐induced Chromospheric Activity on HD 179949","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":246,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Planet; Ephemeris; Astrophysics; Orbit (dynamics); Astronomy; Tidal locking; Exoplanet; Spectral line; Stellar rotation; Rotation period; Satellite; Stars; Radiative transfer","score_opus":0.047260698928874426,"score_gpt":0.27637905833812293,"score_spread":0.22911835940924852,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076572859","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983342,0.00003561843,0.000037206883,0.000017370148,0.0000035035246,0.0000030432125,0.00020756607,0.000006766294,0.0013547207],"genre_scores_gemma":[0.99909174,0.000033445052,0.00009762241,0.000017798873,0.0000076238125,0.000004046398,0.0004463829,0.0000039378538,0.00029735654],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991226,0.000009930758,0.0000062601393,0.000025211528,0.000023027185,0.000023265342],"domain_scores_gemma":[0.99968433,0.000044105673,0.000091117465,0.000037097154,0.000066890054,0.00007647795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009825997,0.00012858488,0.00018303312,0.0005075582,0.0005174599,0.00039550164,0.00023243559,0.0002367928,0.0017761539],"category_scores_gemma":[0.00040532392,0.00011772326,0.0001271138,0.00044073918,0.00030725406,0.00017750243,0.00041792446,0.00020127995,0.00036291877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040690554,0.0001428509,0.7798831,0.00006118453,0.00009998722,0.0010369839,0.00041399663,0.00017560842,0.20818926,0.0002688794,0.0004978194,0.008823328],"study_design_scores_gemma":[0.000007452225,0.000033621425,0.99526334,0.0000028320328,0.000009881147,0.00029441324,0.000050483824,0.00006119266,0.0035808706,0.000026462947,0.0006666182,0.0000027016774],"about_ca_topic_score_codex":0.0024413073,"about_ca_topic_score_gemma":0.004705678,"teacher_disagreement_score":0.0024413073,"about_ca_system_score_codex":0.00029086103,"about_ca_system_score_gemma":0.000115663504,"threshold_uncertainty_score":0.005941868},"labels":[],"label_agreement":null},{"id":"W2076647829","doi":"10.1088/0004-637x/713/2/992","title":"DUST ABUNDANCE AND PROPERTIES IN THE NEARBY DWARF GALAXIES NGC 147 AND NGC 185","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Spitzer Space Telescope; Spectral energy distribution; Infrared; Star formation; Dwarf galaxy; RADIUS; Stars; Luminous infrared galaxy; Stellar mass","score_opus":0.008254955237064014,"score_gpt":0.2011313370257092,"score_spread":0.1928763817886452,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076647829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995809,0.00007607042,0.000035798013,0.0000034248294,6.280315e-7,7.521386e-7,0.00005840442,0.0000071913137,0.00023673131],"genre_scores_gemma":[0.9995042,0.000030754567,0.00010195703,0.0000050800113,0.00000194582,0.0000014077277,0.00025074361,0.0000024916935,0.00010154947],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999571,0.0000026191738,0.0000033045578,0.000012859423,0.000012090268,0.0000120330415],"domain_scores_gemma":[0.99985504,0.00001753163,0.00005014054,0.000013151539,0.000017164622,0.000046939273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000699407,0.00011767388,0.00016909621,0.0005958501,0.00021286849,0.0002944786,0.00015215542,0.00012422809,0.00046422498],"category_scores_gemma":[0.00019142346,0.00008698793,0.00014196298,0.00022204196,0.00019675701,0.00011715236,0.00021845296,0.000110527675,0.0001375001],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024504997,0.00006429175,0.9120604,0.00003289563,0.000053177577,0.0005353739,0.0006203745,0.00026774468,0.07977482,0.00020351348,0.00023358474,0.0059088427],"study_design_scores_gemma":[0.0000020406349,0.000025398038,0.9985911,0.0000010785599,0.0000057341595,0.00022813221,0.00007324097,0.000121062265,0.0007583289,0.000012622932,0.00017966771,0.0000016092089],"about_ca_topic_score_codex":0.0048426534,"about_ca_topic_score_gemma":0.0066725584,"teacher_disagreement_score":0.0048426534,"about_ca_system_score_codex":0.000274265,"about_ca_system_score_gemma":0.000054145225,"threshold_uncertainty_score":0.009628892},"labels":[],"label_agreement":null},{"id":"W2076744870","doi":"10.1086/498347","title":"Compact H<scp>i</scp>Clouds at High Forbidden Velocities in the Inner Galaxy","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Calgary","funders":"","keywords":"Physics; Astrophysics; Longitude; Galactic plane; Galaxy; Latitude; Galactic Center; Astronomy","score_opus":0.0076796398344542586,"score_gpt":0.2056801381494097,"score_spread":0.19800049831495542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2076744870","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991314,0.00017255521,0.0001397556,0.000017429453,0.0000013950245,0.0000029435744,0.00014785914,0.0000110957735,0.00037555853],"genre_scores_gemma":[0.9995677,0.000043770266,0.00008141211,0.000004723827,0.0000036385777,9.551183e-7,0.00024075461,0.0000016899219,0.00005523401],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977463,0.000028081153,0.000009310301,0.000055392,0.000060836268,0.00007182827],"domain_scores_gemma":[0.99909043,0.00014962861,0.00041100435,0.00006447253,0.00006653852,0.00021783255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035435223,0.00024341565,0.00031393324,0.0013171384,0.0004982836,0.0012702758,0.00037098696,0.00028491643,0.0008039495],"category_scores_gemma":[0.0006571506,0.00018591173,0.00015598162,0.0016378483,0.0005937628,0.00035288374,0.0004648159,0.00021177327,0.00024820786],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010812022,0.000029276169,0.98774594,0.000022434362,0.000052382944,0.00023460783,0.00017460664,0.00043343095,0.0055581927,0.00029330316,0.00027410052,0.005073567],"study_design_scores_gemma":[0.0000051740058,0.000030414107,0.9983785,0.0000050891485,0.000014057835,0.0001528754,0.00011029625,0.0005991264,0.00035348424,0.00007719271,0.00027130765,0.0000023824782],"about_ca_topic_score_codex":0.014888588,"about_ca_topic_score_gemma":0.01530925,"teacher_disagreement_score":0.014888588,"about_ca_system_score_codex":0.0006248453,"about_ca_system_score_gemma":0.00026638847,"threshold_uncertainty_score":0.029603839},"labels":[],"label_agreement":null},{"id":"W2077047851","doi":"10.1086/506601","title":"Rotochemical Heating of Neutron Stars: Rigorous Formalism with Electrostatic Potential Perturbations","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Formalism (music); Neutron; Electric potential; Neutron star","score_opus":0.004594403255132466,"score_gpt":0.2612805456258902,"score_spread":0.25668614237075776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077047851","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.21237883,0.008312175,0.60052747,0.0056247897,0.0012027638,0.0001410169,0.0005752543,0.00032869785,0.170909],"genre_scores_gemma":[0.9112072,0.0043453807,0.039583616,0.00083306996,0.0009968493,0.0002695035,0.00033936356,0.00029881686,0.042126283],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.999729,0.00013277831,0.000011161797,0.000021476142,0.00006768181,0.000037882797],"domain_scores_gemma":[0.9995684,0.00012460058,0.000062343766,0.000065058026,0.000091853864,0.00008771011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009827178,0.00092612096,0.0009671375,0.00082848326,0.0007115192,0.0015530969,0.001249707,0.001190921,0.002426225],"category_scores_gemma":[0.0018712726,0.00039049663,0.0008881887,0.000502822,0.001835445,0.0018226063,0.0021512706,0.0011570211,0.0005223064],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003466191,0.00002967404,0.00043295894,0.00006591697,0.000034688564,0.00013193047,0.000114653354,0.10216314,0.0010637719,0.8917879,0.001442847,0.0026978615],"study_design_scores_gemma":[0.00002744319,0.000019605808,0.00033584953,0.000019041294,0.000008635894,0.000047626192,0.000054529282,0.5728404,0.00012079277,0.4242246,0.0022827883,0.000018596867],"about_ca_topic_score_codex":0.0037980606,"about_ca_topic_score_gemma":0.0031025654,"teacher_disagreement_score":0.0037980606,"about_ca_system_score_codex":0.000967444,"about_ca_system_score_gemma":0.00085716567,"threshold_uncertainty_score":0.008116543},"labels":[],"label_agreement":null},{"id":"W2077102027","doi":"10.1088/0004-637x/794/1/67","title":"THE REDSHIFT EVOLUTION OF THE MEAN TEMPERATURE, PRESSURE, AND ENTROPY PROFILES IN 80 SPT-SELECTED GALAXY CLUSTERS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Space Telescope Science Institute; Smithsonian Astrophysical Observatory; McGill University; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; University of Chicago; Smithsonian Institution; National Science Foundation","keywords":"Redshift; Galaxy cluster; Galaxy; Entropy (arrow of time); Telescope; Galaxy groups and clusters; Cosmology","score_opus":0.003317123242901356,"score_gpt":0.18688874016789475,"score_spread":0.1835716169249934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077102027","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997353,0.000010379745,0.00003155821,0.0000043147656,2.247102e-7,8.7148726e-7,0.00014714885,0.000006606947,0.00006346841],"genre_scores_gemma":[0.9990777,0.000014649922,0.00010863484,0.000002620349,0.0000018954402,0.0000031770514,0.00068522,0.000005121331,0.000101014884],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983335,0.000020920857,0.000008615932,0.00005668815,0.00003378908,0.00004674697],"domain_scores_gemma":[0.9987368,0.00025130203,0.0003738195,0.00014836651,0.00019858952,0.0002910518],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034228674,0.00026045027,0.0004074581,0.0014053168,0.00040503364,0.00056961813,0.00030558335,0.0002926772,0.0010193692],"category_scores_gemma":[0.0014913091,0.0002750774,0.0002676351,0.00095795497,0.00041587141,0.00029105577,0.00068272994,0.0002051109,0.00031669255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029637618,0.000027382059,0.982842,0.000011841317,0.000078678124,0.0001381877,0.00046562575,0.0028041287,0.009463068,0.0001129196,0.00024949358,0.0035102707],"study_design_scores_gemma":[0.000002546064,0.000023634842,0.9980513,5.500592e-7,0.000007120587,0.00004778728,0.00006626817,0.0014020157,0.00030639258,0.000022366627,0.00006612272,0.000003966194],"about_ca_topic_score_codex":0.010005048,"about_ca_topic_score_gemma":0.008552781,"teacher_disagreement_score":0.010005048,"about_ca_system_score_codex":0.000503032,"about_ca_system_score_gemma":0.00014301924,"threshold_uncertainty_score":0.019893646},"labels":[],"label_agreement":null},{"id":"W2077143832","doi":"10.1086/498387","title":"A Massive Jet Ejection Event from the Microquasar SS 433 Accompanying Rapid X‐Ray Variability","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Jet (fluid); Astrophysics; Event (particle physics); Kinetic energy; Plasma; Binary number; Nuclear physics; Mechanics","score_opus":0.010544299651571226,"score_gpt":0.22454381751070485,"score_spread":0.21399951785913363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077143832","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981439,0.00018249189,0.00054186163,0.000025142976,0.000008089857,0.000008818736,0.00008228833,0.000028557068,0.0009789416],"genre_scores_gemma":[0.998904,0.00008944284,0.0004789985,0.000021031901,0.000011759388,0.000003405222,0.00018499982,0.000004200487,0.00030213082],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994516,0.00000408755,0.0000052437103,0.000012831217,0.000017912866,0.000014786763],"domain_scores_gemma":[0.9997311,0.00002822919,0.00013254998,0.000031245407,0.00001400933,0.000062830746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011828645,0.00020607028,0.00019057188,0.00034304743,0.00030608109,0.00042379848,0.00013661076,0.00038213033,0.00071046385],"category_scores_gemma":[0.00031781135,0.0001257823,0.00019327765,0.0003265883,0.00019028535,0.00020322883,0.00055916625,0.00027555772,0.00017264594],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009150198,0.00008813092,0.33385518,0.00016592421,0.000111866044,0.019753443,0.0007010567,0.0006601299,0.61287904,0.001272853,0.0006351899,0.028962294],"study_design_scores_gemma":[0.00002041521,0.0003305593,0.9583857,0.000011650199,0.000038190898,0.013615652,0.00015206967,0.000885014,0.023241151,0.000379474,0.002921016,0.00001920315],"about_ca_topic_score_codex":0.0004262751,"about_ca_topic_score_gemma":0.0006851677,"teacher_disagreement_score":0.00071046385,"about_ca_system_score_codex":0.00009620648,"about_ca_system_score_gemma":0.00007176515,"threshold_uncertainty_score":0.0023767352},"labels":[],"label_agreement":null},{"id":"W2077148818","doi":"10.1088/0004-637x/778/1/14","title":"GALAXY CLUSTER BARYON FRACTIONS REVISITED","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":310,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Baryon; Halo; Galaxy; Stellar mass; Galaxy cluster; Cluster (spacecraft); Stars","score_opus":0.006567596734446697,"score_gpt":0.21315164515395302,"score_spread":0.2065840484195063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077148818","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889498,0.00050459494,0.0008584951,0.00006433584,0.000008934172,0.000007866038,0.001894482,0.00012885522,0.0075825904],"genre_scores_gemma":[0.9981895,0.000059418737,0.00029872588,0.000013034638,0.0000071191353,0.0000025319143,0.0009606398,0.0000106159005,0.00045847398],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998018,0.000020696634,0.0000089264695,0.000058037946,0.000050563795,0.000060011414],"domain_scores_gemma":[0.9993925,0.00009714788,0.00018183293,0.00011119348,0.00009876699,0.00011860632],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027344702,0.0002632323,0.00023823757,0.0022302438,0.00036305288,0.0007208146,0.00032830995,0.00019659162,0.002474568],"category_scores_gemma":[0.0012572131,0.00008797958,0.0001880377,0.001939517,0.0003323719,0.00033210398,0.0007330886,0.0001926712,0.00054589834],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012323738,0.0000115099865,0.973307,0.000036607,0.000108261236,0.000051660594,0.00040304416,0.0017906966,0.0029953155,0.0018795803,0.0012627218,0.018030286],"study_design_scores_gemma":[0.000002909905,0.00001301165,0.99509573,0.0000071115755,0.000018124247,0.00010228162,0.00014681237,0.0013536107,0.0008994994,0.00061253924,0.0017415115,0.0000068335617],"about_ca_topic_score_codex":0.010264604,"about_ca_topic_score_gemma":0.010643413,"teacher_disagreement_score":0.010264604,"about_ca_system_score_codex":0.0005513986,"about_ca_system_score_gemma":0.0001793013,"threshold_uncertainty_score":0.020409703},"labels":[],"label_agreement":null},{"id":"W2077223734","doi":"10.1088/0004-637x/790/2/105","title":"SDSS/SEGUE SPECTRAL FEATURE ANALYSIS FOR STELLAR ATMOSPHERIC PARAMETER ESTIMATION","year":2014,"lang":"pt","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Windsor","funders":"","keywords":"Consistency (knowledge bases); Spectral line; Sky; Young stellar object; Pipeline (software); Astronomical spectroscopy; Estimation theory; Stellar classification","score_opus":0.010160478013186256,"score_gpt":0.23239225326002094,"score_spread":0.22223177524683468,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077223734","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.19240108,0.001212457,0.59605944,0.00052095356,0.00022987115,0.00021801841,0.101260774,0.102747455,0.005349938],"genre_scores_gemma":[0.3486118,0.0002647372,0.4925545,0.00024763966,0.000106730055,0.00037226896,0.14999238,0.005165193,0.0026847483],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99954635,0.00010152248,0.000028722758,0.00015885776,0.0001223193,0.000042099142],"domain_scores_gemma":[0.9991394,0.00016106929,0.00012556658,0.00036681705,0.00016965017,0.000037570808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012334548,0.0010715087,0.00061497575,0.0024774617,0.0004017925,0.0007377252,0.0012139295,0.0008337406,0.005196906],"category_scores_gemma":[0.003987791,0.000333911,0.0013904189,0.0017422298,0.00019225059,0.0010225022,0.0010974334,0.0012549255,0.0043199435],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082369824,0.000743657,0.12062115,0.0005527012,0.0012527587,0.0004778652,0.0007486437,0.0773059,0.054637466,0.0097827995,0.22369002,0.50936335],"study_design_scores_gemma":[0.00015927944,0.00011640771,0.09604729,0.00006140828,0.00012108551,0.00026695282,0.00029281533,0.7746156,0.021497812,0.017891336,0.08877854,0.0001515419],"about_ca_topic_score_codex":0.004717451,"about_ca_topic_score_gemma":0.0068440046,"teacher_disagreement_score":0.005196906,"about_ca_system_score_codex":0.00026753562,"about_ca_system_score_gemma":0.00046463936,"threshold_uncertainty_score":0.017385364},"labels":[],"label_agreement":null},{"id":"W2077264194","doi":"10.1086/338032","title":"Interstellar Turbulence. II. Energy Spectra of Molecular Regions in the Outer Galaxy","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Spectral line; Interstellar medium; Spectral density; Turbulence; Dissipative system; Proper motion; Line (geometry); Fractal","score_opus":0.01118783210944167,"score_gpt":0.21224144571641004,"score_spread":0.20105361360696838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077264194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903092,0.00015547761,0.0067717885,0.000045323697,0.000007657891,0.000010790545,0.00040971077,0.000101464175,0.0021885927],"genre_scores_gemma":[0.99861264,0.000032247488,0.0008868533,0.0000044096278,0.0000024292017,0.0000028637653,0.00023024964,0.000008599211,0.00021978181],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996376,0.0000034048774,0.000002131492,0.000006834892,0.000010458197,0.000013309496],"domain_scores_gemma":[0.99985003,0.00003135994,0.000044447264,0.000017679797,0.000024425943,0.00003201648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007386216,0.00015341488,0.00009664969,0.0004345031,0.00015443802,0.00033088692,0.00012441087,0.00011983042,0.00059952756],"category_scores_gemma":[0.0004569671,0.00006593497,0.00018101378,0.0003738058,0.00018720263,0.00017526095,0.0001756762,0.00015249588,0.00014117868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043405755,0.0001205858,0.5621839,0.00011620314,0.00017242687,0.00059400103,0.000381614,0.17653103,0.18088642,0.020546036,0.0020772356,0.0559565],"study_design_scores_gemma":[0.000012365693,0.000049456878,0.7874915,0.0000066298776,0.00001627686,0.00017374191,0.000078251214,0.19544294,0.010466328,0.005111843,0.0011329136,0.000017768634],"about_ca_topic_score_codex":0.0043158475,"about_ca_topic_score_gemma":0.0026502046,"teacher_disagreement_score":0.0043158475,"about_ca_system_score_codex":0.00028553506,"about_ca_system_score_gemma":0.00010624493,"threshold_uncertainty_score":0.0085814595},"labels":[],"label_agreement":null},{"id":"W2077276236","doi":"10.1088/0004-637x/737/1/12","title":"THE CO-TO-H<sub>2</sub>CONVERSION FACTOR FROM INFRARED DUST EMISSION ACROSS THE LOCAL GROUP","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":569,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Metallicity; Milky Way; Local Group; Galaxy; Large Magellanic Cloud; Infrared; Small Magellanic Cloud; Interstellar medium; Cosmic dust","score_opus":0.014780004693881394,"score_gpt":0.2388320552897074,"score_spread":0.22405205059582603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077276236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99830735,0.00004084638,0.000995015,0.000009857984,5.532373e-7,0.0000031636066,0.000055421533,0.000025617092,0.00056211144],"genre_scores_gemma":[0.9996344,0.000012101775,0.00024398198,0.0000023974396,0.000001108633,0.0000012553392,0.000049947947,0.0000034027757,0.00005136811],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.99992776,0.000008413022,0.00000255938,0.000030077748,0.000014115279,0.000017210867],"domain_scores_gemma":[0.99956554,0.00007449685,0.00019157723,0.000059593378,0.000050688657,0.000058139554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001424252,0.00034967987,0.0001232913,0.00043545951,0.00017388967,0.0003120804,0.00027373707,0.0002135334,0.00095066155],"category_scores_gemma":[0.00060085295,0.00013774326,0.00023748422,0.0003290225,0.00022480036,0.00024684236,0.00017271379,0.00012927002,0.00024501648],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007642348,0.000016855387,0.96393913,0.00001729751,0.000046231948,0.00007940352,0.00009811808,0.011788917,0.015372186,0.00038505855,0.00011142277,0.008068841],"study_design_scores_gemma":[0.0000075495363,0.000063134976,0.9602272,0.0000056098042,0.000051279498,0.00016621388,0.000098248915,0.03309486,0.00532233,0.00040078044,0.00055628637,0.0000065076665],"about_ca_topic_score_codex":0.01154048,"about_ca_topic_score_gemma":0.0103665525,"teacher_disagreement_score":0.01154048,"about_ca_system_score_codex":0.00049357675,"about_ca_system_score_gemma":0.00008536123,"threshold_uncertainty_score":0.022946596},"labels":[],"label_agreement":null},{"id":"W2077403383","doi":"10.1086/509063","title":"Temporal Evolution of Coronagraphic Dynamic Range and Constraints on Companions to Vega","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Speckle pattern; Physics; Adaptive optics; Telescope; Speckle imaging; Vega; Limiting magnitude; Brightness; Stars; Astrophysics; Interferometry; Optics; Astronomy","score_opus":0.007217896709829286,"score_gpt":0.21661276312171804,"score_spread":0.20939486641188876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077403383","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99838877,0.0001564977,0.00024567373,0.000030822044,0.000002552267,0.000002618497,0.0003127461,0.000017315539,0.00084315275],"genre_scores_gemma":[0.99867237,0.000040335268,0.00019868431,0.000010774422,0.0000048614493,0.0000039937554,0.0009180689,0.000007673814,0.00014336828],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978775,0.000022634265,0.000012492083,0.000081473845,0.000033393106,0.00006229195],"domain_scores_gemma":[0.99858594,0.00039241632,0.00039284918,0.0001511994,0.00025035776,0.00022727349],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004034127,0.0001292964,0.00026623916,0.001583266,0.0004437215,0.0007942281,0.00030675388,0.0003604122,0.00083234033],"category_scores_gemma":[0.0025822695,0.000193208,0.00014989999,0.00076979893,0.00027948446,0.00044112233,0.0006502325,0.00029220074,0.00025088043],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010149854,0.00003754232,0.9792255,0.000016152728,0.00004434946,0.00013246023,0.00035079048,0.0007557459,0.012943291,0.00019747381,0.00034959335,0.00584556],"study_design_scores_gemma":[0.0000010699563,0.00001048104,0.9983246,0.0000035213043,0.0000053908357,0.00009039526,0.000088722896,0.0008270392,0.00024713288,0.00003310208,0.00036517746,0.0000034120767],"about_ca_topic_score_codex":0.007953337,"about_ca_topic_score_gemma":0.017188763,"teacher_disagreement_score":0.007953337,"about_ca_system_score_codex":0.00039967368,"about_ca_system_score_gemma":0.00013678164,"threshold_uncertainty_score":0.015814126},"labels":[],"label_agreement":null},{"id":"W2077448604","doi":"10.1086/430939","title":"An Unusual System of H<scp>i</scp>Filaments near WR 5 and HD 17603","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Defence Research and Development Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Stars; Physics; Astrophysics; Context (archaeology); Wolf–Rayet star; Spiral galaxy; Molecular cloud; Galaxy; Star formation; Astronomy; Geology","score_opus":0.008241618945908668,"score_gpt":0.2372208819569623,"score_spread":0.22897926301105365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077448604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975001,0.000116650146,0.00025533707,0.000023419909,0.0000036533268,0.000005561167,0.00008993287,0.000025161216,0.0019801082],"genre_scores_gemma":[0.999328,0.000017563914,0.00043261633,0.000010501714,0.000004351331,0.0000021316714,0.00008719576,0.000001475766,0.00011617839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999299,0.0000046304804,0.000004666816,0.000022750959,0.000018482857,0.000019594641],"domain_scores_gemma":[0.99971,0.000022679134,0.00015118723,0.00003469042,0.000027646116,0.000053664844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007927384,0.000107384585,0.00010592668,0.00063050573,0.00043455054,0.0005365632,0.00038835497,0.00024705663,0.0008323741],"category_scores_gemma":[0.0003731398,0.00013248414,0.000086393804,0.00053261267,0.0003323155,0.00018866915,0.0003236018,0.00015156204,0.00015836522],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004241889,0.00006422987,0.595466,0.00010736556,0.0001152982,0.020609386,0.0009650348,0.0008378245,0.35451198,0.0024079185,0.0010642848,0.023426432],"study_design_scores_gemma":[0.000027771535,0.000113143135,0.95681113,0.000022799104,0.00005842713,0.017090095,0.00038483657,0.0012361325,0.018410746,0.00079825125,0.005029496,0.00001720215],"about_ca_topic_score_codex":0.0023535844,"about_ca_topic_score_gemma":0.0033736741,"teacher_disagreement_score":0.0023535844,"about_ca_system_score_codex":0.0002339339,"about_ca_system_score_gemma":0.00012921802,"threshold_uncertainty_score":0.004679799},"labels":[],"label_agreement":null},{"id":"W2077460073","doi":"10.1086/319067","title":"Deprojecting Sunyaev‐Zeldovich Statistics","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Spectral density; Skewness; Galaxy; Redshift; Intergalactic travel; Anisotropy; Perturbation theory (quantum mechanics); Spectral line; Cosmology","score_opus":0.010384455888643883,"score_gpt":0.2340095795677342,"score_spread":0.2236251236790903,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077460073","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14434892,0.00029171005,0.8434808,0.00029184972,0.00008476788,0.00005816052,0.0004955997,0.0008969182,0.010051317],"genre_scores_gemma":[0.92312586,0.00069099205,0.055217557,0.00012391205,0.0001357123,0.00012300193,0.000855234,0.0005168884,0.019210955],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994773,0.00014058841,0.000026454503,0.0000855602,0.00015856302,0.000111492074],"domain_scores_gemma":[0.997517,0.0008394548,0.00040042782,0.00075217534,0.00033243268,0.00015856563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017018846,0.0007430246,0.00075001444,0.0016524979,0.00046011552,0.0015199583,0.0015146327,0.00045198185,0.0038641267],"category_scores_gemma":[0.006040741,0.00042031048,0.00087223836,0.0011203763,0.0009797945,0.0015281833,0.0010702845,0.0009833908,0.0013741913],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043570373,0.000031565236,0.004253414,0.000043946453,0.0000494963,0.00022922944,0.00008792094,0.4790386,0.002353929,0.49837962,0.001465454,0.014023313],"study_design_scores_gemma":[0.000005189131,0.0000102076565,0.0008085209,0.0000045704955,0.000007917681,0.000044713335,0.000009792185,0.9277818,0.0010161492,0.06954212,0.00075296307,0.000016020595],"about_ca_topic_score_codex":0.013437848,"about_ca_topic_score_gemma":0.00911318,"teacher_disagreement_score":0.013437848,"about_ca_system_score_codex":0.0012326902,"about_ca_system_score_gemma":0.0010449756,"threshold_uncertainty_score":0.026719213},"labels":[],"label_agreement":null},{"id":"W2077466198","doi":"10.1088/0004-637x/784/1/57","title":"CHARACTERIZATION OF THE PRAESEPE STAR CLUSTER BY PHOTOMETRY AND PROPER MOTIONS WITH 2MASS, PPMXL, AND Pan-STARRS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Mass segregation; Photometry (optics); Cluster (spacecraft); Open cluster; Astronomy; Stars; Stellar mass; Sky; Proper motion; Stellar density; Star cluster; Population; Mass ratio; Blue straggler; Stellar population; Star formation","score_opus":0.005099306838797556,"score_gpt":0.18881759341482798,"score_spread":0.18371828657603043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077466198","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972959,0.00002427282,0.00096704735,0.000013822457,0.0000013986024,0.000016174103,0.00021027651,0.000020943524,0.0014500269],"genre_scores_gemma":[0.99457896,0.000040113624,0.0027280662,0.000008463381,0.000004426068,0.000024300509,0.001056634,0.000012591101,0.0015464775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985945,0.0000123666405,0.0000092832415,0.00004848888,0.00004710783,0.000023269726],"domain_scores_gemma":[0.9996613,0.000045891506,0.00007814542,0.00007089389,0.00007570215,0.00006801628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002672381,0.00015184685,0.00020504522,0.0011059401,0.00050391885,0.0003566589,0.00030192581,0.00012213977,0.0023094488],"category_scores_gemma":[0.0010595436,0.000099592035,0.000109254615,0.00049655396,0.00021090578,0.00038368517,0.0008449217,0.00020644275,0.0008435646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017181596,0.000037798683,0.94439477,0.000031347954,0.00002471262,0.00032968834,0.0007095037,0.00090209045,0.027099602,0.0010849994,0.0005750135,0.024638731],"study_design_scores_gemma":[0.0000059030062,0.00008279385,0.99031395,0.0000047222115,0.0000061784854,0.0005651324,0.00029180228,0.0024939664,0.0026196784,0.00022103431,0.0033888891,0.000005881804],"about_ca_topic_score_codex":0.0030317728,"about_ca_topic_score_gemma":0.0050538927,"teacher_disagreement_score":0.0030317728,"about_ca_system_score_codex":0.00015864332,"about_ca_system_score_gemma":0.00021484206,"threshold_uncertainty_score":0.007725835},"labels":[],"label_agreement":null},{"id":"W2077579588","doi":"10.1088/0004-637x/728/1/55","title":"LOW-IONIZATION LINE EMISSION FROM A STARBURST GALAXY: A NEW PROBE OF A GALACTIC-SCALE OUTFLOW","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Emission spectrum; Galaxy; Surface brightness; Line (geometry); Stars; Outflow; Brightness; Spectroscopy; Spectral line","score_opus":0.01130407654825461,"score_gpt":0.20802327035684362,"score_spread":0.19671919380858902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077579588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99872655,0.0001117532,0.00047139882,0.000016613561,0.000001024,0.0000017816263,0.00005076381,0.000021724572,0.00059829303],"genre_scores_gemma":[0.99914694,0.000055860393,0.00052739604,0.000018457415,0.000004589146,0.0000017697204,0.00010697762,0.0000046614496,0.00013326434],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996424,0.000003581791,0.0000017314429,0.00001326624,0.0000066776797,0.0000104384835],"domain_scores_gemma":[0.9998367,0.000024809364,0.00007035534,0.000013132321,0.000013562826,0.00004147463],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000876046,0.00015705122,0.00013787192,0.00044139195,0.0002206678,0.00038677937,0.00019749776,0.00026969917,0.0005964297],"category_scores_gemma":[0.00015765814,0.00012401551,0.000083320025,0.00027138944,0.00021082556,0.00028660422,0.00024389282,0.00022328965,0.00014383736],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002493875,0.00012683237,0.55698556,0.00006271488,0.000045080254,0.00046316982,0.00037758626,0.0004126245,0.43063948,0.00038143154,0.00016036231,0.010095751],"study_design_scores_gemma":[0.000014780297,0.000151624,0.98675215,0.0000072867715,0.000021664242,0.0006564218,0.000103584236,0.0011365729,0.010267107,0.00022600163,0.00065675616,0.0000059700146],"about_ca_topic_score_codex":0.00070564455,"about_ca_topic_score_gemma":0.0015714436,"teacher_disagreement_score":0.00070564455,"about_ca_system_score_codex":0.00013040457,"about_ca_system_score_gemma":0.000049242837,"threshold_uncertainty_score":0.0019952655},"labels":[],"label_agreement":null},{"id":"W2077684395","doi":"10.1088/0004-637x/704/2/1135","title":"A RELATIONSHIP BETWEEN SUPERMASSIVE BLACK HOLE MASS AND THE TOTAL GRAVITATIONAL MASS OF THE HOST GALAXY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Supermassive black hole; Black hole (networking); Galaxy; Velocity dispersion; Stellar black hole; Stellar mass; Spin-flip; RADIUS; Gravitation","score_opus":0.009410106768227329,"score_gpt":0.21900795795342703,"score_spread":0.20959785118519972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077684395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982823,0.00015804527,0.0005141569,0.00003828761,0.0000012681128,0.000002381056,0.00011216989,0.000022338716,0.000869002],"genre_scores_gemma":[0.9995852,0.000025702038,0.000196749,0.000007973883,0.000004999322,0.0000011341687,0.00008591663,0.0000025413806,0.00008989099],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980825,0.00004856225,0.00001299781,0.000050326464,0.00004313288,0.00003673699],"domain_scores_gemma":[0.99260384,0.0025139444,0.0034032147,0.00055043265,0.00041076847,0.0005178293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005346386,0.0003188219,0.00018783557,0.00085141225,0.00016314907,0.00053606427,0.0002748857,0.00026886864,0.0018434005],"category_scores_gemma":[0.004334055,0.00018712481,0.00025087374,0.0007149582,0.00048851396,0.00047569783,0.0004225959,0.0002795772,0.00037685302],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033825,0.000007959487,0.99556607,0.0000058526825,0.00004991218,0.000056882567,0.000031338404,0.000529237,0.0018453583,0.00023711697,0.00005205913,0.0015844225],"study_design_scores_gemma":[0.000004321715,0.00004625004,0.99508923,0.0000031806094,0.000017290999,0.00015868164,0.000048310365,0.0034712134,0.0006607805,0.00037532678,0.00012077702,0.0000046195178],"about_ca_topic_score_codex":0.002707246,"about_ca_topic_score_gemma":0.0038078534,"teacher_disagreement_score":0.002707246,"about_ca_system_score_codex":0.00018859738,"about_ca_system_score_gemma":0.0001677962,"threshold_uncertainty_score":0.006166756},"labels":[],"label_agreement":null},{"id":"W2077693547","doi":"10.1088/0004-637x/757/1/47","title":"OHMIC DISSIPATION IN THE INTERIORS OF HOT JUPITERS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Hot Jupiter; Ohmic contact; Joule heating; Convection; Planet; Magnetic field; Dissipation; Gas giant","score_opus":0.01256534328202969,"score_gpt":0.2418302123973531,"score_spread":0.22926486911532343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077693547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9689316,0.00027055712,0.014709348,0.00029199905,0.00003250619,0.000018263294,0.00007400557,0.00016043852,0.01551131],"genre_scores_gemma":[0.9979547,0.00007749991,0.0007015507,0.000028599457,0.000014662331,0.000011709891,0.000022728529,0.000027233687,0.0011613934],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998994,0.000027239566,0.0000030609226,0.000017588494,0.000015005762,0.000037700243],"domain_scores_gemma":[0.99967265,0.00007165448,0.00008426697,0.00005661605,0.000022023227,0.000092758564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023982629,0.00055662263,0.00053600554,0.0003686831,0.00086684996,0.0011638076,0.00092836097,0.0009115213,0.0014334783],"category_scores_gemma":[0.0014822446,0.0005036377,0.0007470584,0.00022549868,0.001827542,0.001437062,0.0016398623,0.0007506944,0.00021507897],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024106969,0.00008426128,0.012686701,0.00005697425,0.000057799647,0.0010103999,0.000780848,0.9220887,0.011628417,0.04743238,0.00076221355,0.003170225],"study_design_scores_gemma":[0.00016163662,0.00015497742,0.01097281,0.000021822441,0.00004468541,0.0002726743,0.0002157953,0.9527727,0.0013064853,0.032407653,0.0016260332,0.000042705207],"about_ca_topic_score_codex":0.0043137376,"about_ca_topic_score_gemma":0.0017832766,"teacher_disagreement_score":0.0043137376,"about_ca_system_score_codex":0.0008194221,"about_ca_system_score_gemma":0.0002761463,"threshold_uncertainty_score":0.008577228},"labels":[],"label_agreement":null},{"id":"W2077719548","doi":"10.1088/0004-637x/723/1/197","title":"GALAXY EVOLUTION IN A COMPLEX ENVIRONMENT: A MULTI-WAVELENGTH STUDY OF HCG 7","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Western University","funders":"","keywords":"Dwarf galaxy; Galaxy; Globular cluster; Galaxy merger; Hubble space telescope; Star formation; Stars; Lenticular galaxy; Elliptical galaxy; Galaxy formation and evolution","score_opus":0.012738669353335218,"score_gpt":0.2234834970744635,"score_spread":0.21074482772112826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077719548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996402,0.000022459544,0.000050343784,0.000008472623,5.3801244e-7,0.0000015022882,0.00003228612,0.000002481645,0.00024162435],"genre_scores_gemma":[0.9993345,0.00002792842,0.00024358428,0.000015108426,0.000002918123,0.0000018447282,0.0001552111,0.0000057207576,0.00021314334],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998785,0.00001992823,0.000004356602,0.000025280016,0.000026701933,0.000045150344],"domain_scores_gemma":[0.99960893,0.00004709104,0.00008771033,0.00004664933,0.0000561685,0.00015353425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017124318,0.00012576372,0.00021442988,0.000669191,0.00035852927,0.000444374,0.00022320259,0.0001727459,0.0005539126],"category_scores_gemma":[0.00041536248,0.00008240549,0.00019972265,0.0005318553,0.0003758814,0.00024230166,0.0006943379,0.00028025024,0.00019441845],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000083611245,0.00014265554,0.9601083,0.000013471976,0.00006458142,0.001114746,0.001231106,0.0008163176,0.029112456,0.00034387628,0.00024700133,0.006721948],"study_design_scores_gemma":[0.0000017421326,0.000057718968,0.99721754,0.0000021580174,0.000010176749,0.0002568013,0.0005480262,0.00054460735,0.00080354564,0.00008957807,0.00046410816,0.000003962314],"about_ca_topic_score_codex":0.006287065,"about_ca_topic_score_gemma":0.0087759765,"teacher_disagreement_score":0.006287065,"about_ca_system_score_codex":0.00033134842,"about_ca_system_score_gemma":0.0001507306,"threshold_uncertainty_score":0.012500942},"labels":[],"label_agreement":null},{"id":"W2077736421","doi":"10.1086/318314","title":"A Survey of Organic Volatile Species in Comet C/1999 H1 (Lee) Using NIRSPEC at the Keck Observatory","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of New Brunswick","funders":"","keywords":"Comet; Physics; Observatory; Carbon monoxide; Astrobiology; Astrophysics; Infrared; Methane; Astronomy; Acetylene; Chemistry; Organic chemistry","score_opus":0.0382764916020165,"score_gpt":0.2375604428395973,"score_spread":0.1992839512375808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077736421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992631,0.000112413385,0.000030542546,0.000009091483,8.6133053e-7,0.0000037837763,0.00029502952,0.000005193636,0.00028002285],"genre_scores_gemma":[0.9968856,0.00022711877,0.00031582307,0.000032556494,0.000010377674,0.000007677088,0.0020669138,0.000006300383,0.0004476691],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988604,0.0000054714733,0.00000497125,0.000032619435,0.000036572543,0.0000343063],"domain_scores_gemma":[0.99972755,0.000022410732,0.00009504875,0.00001691304,0.0000646129,0.00007335964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001481136,0.00025993105,0.00018788644,0.0016532188,0.00056401745,0.00035299378,0.00019511745,0.00032054877,0.00052116986],"category_scores_gemma":[0.00022055462,0.00014901528,0.00013818253,0.00059906574,0.00017640472,0.0002849015,0.0002952185,0.00020651007,0.00017202152],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003213984,0.00014311235,0.67894506,0.000075683434,0.000096154596,0.00082555006,0.0007977843,0.00012932306,0.30756053,0.000054413376,0.00025888215,0.01079204],"study_design_scores_gemma":[0.0000031680786,0.00005684171,0.9932781,0.0000023398852,0.000010141477,0.000249641,0.00006953627,0.000069037524,0.0058331573,0.000004570158,0.00042019284,0.0000032715445],"about_ca_topic_score_codex":0.0061439797,"about_ca_topic_score_gemma":0.013916238,"teacher_disagreement_score":0.0061439797,"about_ca_system_score_codex":0.00048164075,"about_ca_system_score_gemma":0.00014741757,"threshold_uncertainty_score":0.012216449},"labels":[],"label_agreement":null},{"id":"W2077749088","doi":"10.1086/521996","title":"Hot Jupiters in Binary Star Systems","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":202,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Hot Jupiter; Planet; Planetary system; Binary star; Orbit (dynamics); Eccentricity (behavior); Radial velocity; Mass distribution; Planetary migration; Jupiter mass","score_opus":0.011356950631005166,"score_gpt":0.2286996424770681,"score_spread":0.21734269184606292,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077749088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9861124,0.0044303546,0.00012330318,0.0001801947,0.000015174441,0.000011127383,0.00014750143,0.000007510482,0.00897235],"genre_scores_gemma":[0.99817336,0.0008197256,0.00006449756,0.000030179164,0.00002883998,0.0000038875164,0.00016648957,0.0000019685838,0.0007110847],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996952,0.000042998312,0.00002620705,0.00008271434,0.00006268628,0.0000902068],"domain_scores_gemma":[0.999419,0.000102091944,0.00024303127,0.000027548807,0.000046140278,0.00016226205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002353397,0.000110255554,0.00028747227,0.0013357094,0.0013531129,0.0019592543,0.00026217656,0.0004569445,0.004903865],"category_scores_gemma":[0.0015419524,0.00016389515,0.000078704325,0.0013434854,0.00065248064,0.0008001526,0.0010095153,0.00028078997,0.00064626307],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026632653,0.00010027033,0.9460778,0.00016089025,0.000038757582,0.0010430661,0.0032354926,0.00024344797,0.0040106354,0.0043418854,0.0015915001,0.03888997],"study_design_scores_gemma":[0.0000065265967,0.000048473827,0.9897928,0.000030047839,0.00001531141,0.0019282709,0.0013668592,0.00019241063,0.00030999607,0.0014164489,0.004887454,0.0000053762456],"about_ca_topic_score_codex":0.004713092,"about_ca_topic_score_gemma":0.004664091,"teacher_disagreement_score":0.004903865,"about_ca_system_score_codex":0.0005363791,"about_ca_system_score_gemma":0.00024139776,"threshold_uncertainty_score":0.016405046},"labels":[],"label_agreement":null},{"id":"W2077759143","doi":"10.1088/0004-637x/719/1/497","title":"THE DIRECTLY IMAGED PLANET AROUND THE YOUNG SOLAR ANALOG 1RXS J160929.1 – 210524: CONFIRMATION OF COMMON PROPER MOTION, TEMPERATURE, AND MASS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto","funders":"","keywords":"Planet; Proper motion; Planetary mass; Physics; Brown dwarf; Astrophysics; Jupiter mass; Photometry (optics); Astronomy; Primary (astronomy); Solar System; Solar mass; Planetary system; Stars; Exoplanet","score_opus":0.006045407814064636,"score_gpt":0.20780585955213082,"score_spread":0.2017604517380662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077759143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964529,0.00016456451,0.00036360146,0.000051989355,0.000011595438,0.000005307964,0.00015316413,0.0000696236,0.0027272515],"genre_scores_gemma":[0.99687046,0.00007188347,0.0015476639,0.00004259552,0.00001963141,0.00000490709,0.0006390897,0.000011271199,0.0007926329],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999113,0.000005476519,0.0000055711707,0.000039579,0.00002631591,0.000011675432],"domain_scores_gemma":[0.9997774,0.000020591506,0.000089039975,0.000032363554,0.000027164544,0.000053474116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001430592,0.0002172157,0.00019950414,0.00046612063,0.00032751652,0.000351984,0.000319704,0.00043912008,0.0018079964],"category_scores_gemma":[0.00036976056,0.00012739119,0.00012599034,0.0002473274,0.00030367987,0.0002619517,0.00036259578,0.00031051043,0.0006773456],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003074623,0.00026302406,0.46363157,0.00016044105,0.00007179591,0.0036041122,0.000537184,0.0006032423,0.5019884,0.0009087507,0.0021876104,0.025736412],"study_design_scores_gemma":[0.000025003259,0.00019102036,0.960893,0.000021732118,0.000033688397,0.004224744,0.00015870418,0.0023835946,0.027474096,0.00015053622,0.00443108,0.000012951199],"about_ca_topic_score_codex":0.0011312368,"about_ca_topic_score_gemma":0.0028634109,"teacher_disagreement_score":0.0018079964,"about_ca_system_score_codex":0.00020115562,"about_ca_system_score_gemma":0.0000860658,"threshold_uncertainty_score":0.0060483217},"labels":[],"label_agreement":null},{"id":"W2077786625","doi":"10.1086/377365","title":"On Large-Scale Magnetic Field Reversals in the Outer Galaxy","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Galaxy; Magnetic field; Pulsar; Astronomy; Galactic plane; RADIUS; Rotation (mathematics); Field (mathematics)","score_opus":0.007050405485415218,"score_gpt":0.21954450908127246,"score_spread":0.21249410359585724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077786625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99716645,0.00020479655,0.00021491863,0.00008505099,0.000002537938,0.0000022232045,0.0000826441,0.0000058194455,0.0022356082],"genre_scores_gemma":[0.99953616,0.00011511766,0.00007822885,0.000018882805,0.000007436004,8.3319367e-7,0.000102523285,0.0000030471842,0.00013788493],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997826,0.000034054836,0.000008260926,0.000042772746,0.00007149703,0.000060865535],"domain_scores_gemma":[0.9966558,0.0008442924,0.0012369701,0.00039844788,0.0006257968,0.0002386861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056479394,0.00016676262,0.00020291556,0.00090938515,0.00041103933,0.00073627837,0.0004688102,0.00025423805,0.0013044544],"category_scores_gemma":[0.0036480404,0.000098410936,0.00009413,0.0008842465,0.0013767049,0.0006361594,0.0006123623,0.00031817728,0.00027112826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036318225,0.00002815877,0.9598892,0.00003503413,0.00005227887,0.00030174034,0.0010266653,0.0006471504,0.01278014,0.0011139277,0.00030044786,0.023462098],"study_design_scores_gemma":[0.000002700437,0.000016659478,0.9982868,0.0000047029857,0.000010118198,0.00006658005,0.00021997635,0.00019980255,0.0005018396,0.00028026063,0.0004063703,0.00000421122],"about_ca_topic_score_codex":0.051385023,"about_ca_topic_score_gemma":0.071688086,"teacher_disagreement_score":0.051385023,"about_ca_system_score_codex":0.0006247733,"about_ca_system_score_gemma":0.00036203602,"threshold_uncertainty_score":0.10217184},"labels":[],"label_agreement":null},{"id":"W2077842149","doi":"10.1086/508802","title":"Power Laws and Non–Power Laws in Dark Matter Halos","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Dark matter; Power law; Halo; Velocity dispersion; Instability; Cosmology; Dispersion (optics); Phase space; Parameter space; Scalar field dark matter","score_opus":0.0030850040386081307,"score_gpt":0.19697567570666566,"score_spread":0.19389067166805754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077842149","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8788868,0.0004643824,0.11548928,0.00028808572,0.000015886733,0.000035568868,0.00012153657,0.00033940034,0.004359059],"genre_scores_gemma":[0.99396694,0.00018477405,0.0047200746,0.000039010472,0.000016746688,0.000015254489,0.00008247404,0.00007463717,0.0009001721],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996879,0.000130337,0.000014713592,0.000055026707,0.00006177674,0.00005039475],"domain_scores_gemma":[0.9956642,0.0025176418,0.0007878011,0.0005564803,0.00023358298,0.00024032383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012838434,0.00034221204,0.00034932335,0.0010116961,0.00032104884,0.0014050604,0.00084681495,0.0005612952,0.0013157926],"category_scores_gemma":[0.015356009,0.00039866354,0.0004445469,0.00049940124,0.0018482289,0.0021911738,0.0005930462,0.0005415964,0.00021026688],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021945027,0.0000736094,0.06566152,0.00012384464,0.00010400825,0.00082899485,0.00091231783,0.57582957,0.007191042,0.33279172,0.0013704856,0.014893483],"study_design_scores_gemma":[0.000026267457,0.000028450528,0.013341737,0.00001671997,0.000009531949,0.00018655598,0.00008646955,0.83036673,0.0012750167,0.15364224,0.0009943158,0.000025949746],"about_ca_topic_score_codex":0.005300575,"about_ca_topic_score_gemma":0.0022523669,"teacher_disagreement_score":0.005300575,"about_ca_system_score_codex":0.0010467197,"about_ca_system_score_gemma":0.0002035003,"threshold_uncertainty_score":0.010539472},"labels":[],"label_agreement":null},{"id":"W2077858362","doi":"10.1086/343090","title":"Anisotropies in the Motions and Positions of the Galactic Globular Clusters","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Globular cluster; Protein filament; Anisotropy; Galaxy; Ellipsoid; Principal axis theorem; Cluster (spacecraft); Star cluster; Galaxy cluster","score_opus":0.008231363833596132,"score_gpt":0.20004481281410297,"score_spread":0.19181344898050684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077858362","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997426,0.00007025011,0.0006554582,0.000020374408,0.0000024161989,0.00000302842,0.00018954984,0.000010780543,0.0016222422],"genre_scores_gemma":[0.9992567,0.000031633448,0.0002779739,0.0000014542547,0.0000018698073,0.0000019762797,0.0002541447,0.000003560715,0.0001706932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998093,0.000030814725,0.000012010411,0.0000496243,0.000060610902,0.000037592017],"domain_scores_gemma":[0.9993405,0.00019113632,0.00015362687,0.000070930364,0.00016023539,0.00008351011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029863018,0.00015636598,0.00010062386,0.0007446511,0.0002643563,0.00029665485,0.00013452517,0.00009850877,0.0009305545],"category_scores_gemma":[0.0023987475,0.00014196217,0.00010220644,0.00060083956,0.00022901379,0.00018333145,0.00030883498,0.00015324834,0.00024317374],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004995642,0.000017929451,0.8969448,0.000042882242,0.00007718406,0.00009741034,0.0007399854,0.0148498425,0.044316795,0.0040258234,0.0008360567,0.037551776],"study_design_scores_gemma":[0.0000064570227,0.00001836327,0.9869528,0.000004077896,0.00001170597,0.00007964836,0.00015796897,0.009193542,0.001645329,0.0008256945,0.0010904657,0.000014014394],"about_ca_topic_score_codex":0.013785715,"about_ca_topic_score_gemma":0.020264525,"teacher_disagreement_score":0.013785715,"about_ca_system_score_codex":0.00059112575,"about_ca_system_score_gemma":0.0002867365,"threshold_uncertainty_score":0.027410984},"labels":[],"label_agreement":null},{"id":"W2077891330","doi":"10.1086/504146","title":"The Possibly Remnant Massive Outflow in G5.89‐0.39. I. Observations and Initial Magnetohydrodynamic Simulations","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics; McMaster University; University of Calgary","funders":"","keywords":"Outflow; Physics; Magnetohydrodynamic drive; Astrophysics; Jet (fluid); Luminosity; Magnetohydrodynamics; Mechanics; Meteorology; Nuclear physics; Plasma","score_opus":0.011809163794461288,"score_gpt":0.24533149762417908,"score_spread":0.2335223338297178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077891330","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99050564,0.00014972955,0.0008487401,0.00032437738,0.000056755533,0.00002314197,0.0007860552,0.0001633354,0.007142288],"genre_scores_gemma":[0.99827325,0.000030726504,0.00026995176,0.000055320634,0.000014971989,0.0000039469473,0.00038495773,0.000028955146,0.0009379128],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999573,0.000004337886,0.0000026668395,0.00001239936,0.000006395323,0.000016895565],"domain_scores_gemma":[0.99983084,0.000029506553,0.00003242825,0.000011590381,0.000015926187,0.000079696954],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016318393,0.0002701243,0.00046745414,0.0002056663,0.00060838985,0.0009331658,0.00054566393,0.00067959644,0.0035464612],"category_scores_gemma":[0.0002969551,0.00020550577,0.00031559722,0.00017685675,0.00029122506,0.00035252195,0.00054740126,0.00048230667,0.0009685303],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.005125907,0.00088852365,0.4702649,0.0006143698,0.00030947215,0.013576843,0.0010059836,0.23955934,0.18529204,0.017800335,0.023649648,0.04191259],"study_design_scores_gemma":[0.0010038965,0.0005686601,0.5888822,0.00013385183,0.0001603776,0.0011095019,0.00071408955,0.36731982,0.017938571,0.007926474,0.014104935,0.00013763976],"about_ca_topic_score_codex":0.006942056,"about_ca_topic_score_gemma":0.0053695114,"teacher_disagreement_score":0.006942056,"about_ca_system_score_codex":0.0007185825,"about_ca_system_score_gemma":0.0003167348,"threshold_uncertainty_score":0.013803303},"labels":[],"label_agreement":null},{"id":"W2077947153","doi":"10.1088/0004-637x/801/1/26","title":"THE LAST OF<i>FIRST</i>: THE FINAL CATALOG AND SOURCE IDENTIFICATIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":323,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Quest University Canada","funders":"","keywords":"Sky; Galaxy; Astrometry; Flux (metallurgy); Quasar; Active galactic nucleus; Consistency (knowledge bases); Radio galaxy; Luminous infrared galaxy","score_opus":0.020493826385478166,"score_gpt":0.2318497938620297,"score_spread":0.21135596747655153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077947153","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.049355466,0.0039059222,0.021229845,0.008042938,0.006545345,0.0013177516,0.7529366,0.019188046,0.13747804],"genre_scores_gemma":[0.03206654,0.0017726717,0.024028927,0.0035308332,0.0015112142,0.0011194163,0.7627546,0.0035657599,0.1696501],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9988091,0.00006113882,0.00012143436,0.00017259763,0.000564252,0.00027145934],"domain_scores_gemma":[0.99174386,0.00020265325,0.0004116966,0.0018012591,0.004823562,0.0010169361],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015839239,0.0006741905,0.0011022252,0.007370324,0.0013581779,0.0050620493,0.0014814248,0.0008995703,0.080434516],"category_scores_gemma":[0.005655407,0.0004339915,0.0006716513,0.006135774,0.00039873898,0.0027034546,0.0021541426,0.0015400259,0.09443704],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010850545,0.000062039,0.016564718,0.00027085096,0.000022120328,0.000088645764,0.0001263461,0.00011988738,0.0014412338,0.0022877855,0.88249165,0.09641619],"study_design_scores_gemma":[0.000035532335,0.00004580557,0.036397494,0.00014246618,0.000022214988,0.00020691988,0.000120704855,0.0002236013,0.0014174317,0.0009163443,0.9604325,0.0000388603],"about_ca_topic_score_codex":0.016099611,"about_ca_topic_score_gemma":0.02231974,"teacher_disagreement_score":0.080434516,"about_ca_system_score_codex":0.0016897669,"about_ca_system_score_gemma":0.0044616736,"threshold_uncertainty_score":0.26908028},"labels":[],"label_agreement":null},{"id":"W2077974689","doi":"10.1088/0004-637x/747/2/91","title":"THE WiggleZ DARK ENERGY SURVEY: GALAXY EVOLUTION AT 0.25 ⩽<i>z</i>⩽ 0.75 USING THE SECOND RED-SEQUENCE CLUSTER SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Waterloo; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Brightest cluster galaxy; Astronomy; Galaxy cluster; Luminosity function; Galaxy; Luminous infrared galaxy; Luminosity; Cluster (spacecraft)","score_opus":0.02061331553181817,"score_gpt":0.23758921918743348,"score_spread":0.2169759036556153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2077974689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99185,0.00008860877,0.00031689592,0.00003949428,0.0000026205855,0.00001812842,0.005919472,0.000054307176,0.0017105666],"genre_scores_gemma":[0.97870934,0.00012302237,0.0010926315,0.000031521326,0.000007353336,0.000023621084,0.01783456,0.00002692423,0.0021509253],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983966,0.000016068543,0.000007581475,0.000044773788,0.00005158211,0.000040261242],"domain_scores_gemma":[0.99956864,0.000015704429,0.00017033273,0.00006733678,0.000054677992,0.0001233268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022653026,0.00027913932,0.00020689558,0.0017364465,0.00031082053,0.000614965,0.000290315,0.00015394078,0.0012654533],"category_scores_gemma":[0.0003621707,0.00016618056,0.00024216219,0.0017792425,0.00020655715,0.00026399587,0.0006929887,0.00019116991,0.00067172485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011496352,0.000032012784,0.9864095,0.000018438386,0.00007827012,0.00010651793,0.00025757964,0.00045889246,0.005383314,0.00032091845,0.0025091504,0.004310347],"study_design_scores_gemma":[0.0000045833476,0.000008543172,0.9977495,0.0000024982883,0.000007686826,0.00003673179,0.000054888067,0.00027628907,0.00026881488,0.000017210641,0.0015701704,0.000003194302],"about_ca_topic_score_codex":0.1285799,"about_ca_topic_score_gemma":0.30944696,"teacher_disagreement_score":0.1285799,"about_ca_system_score_codex":0.0007549591,"about_ca_system_score_gemma":0.00041639584,"threshold_uncertainty_score":0.25566298},"labels":[],"label_agreement":null},{"id":"W2078020380","doi":"10.1086/339138","title":"Massive Binary WR 112 and Properties of Wolf-Rayet Dust","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Université de Montréal","funders":"","keywords":"Cosmic dust; Binary number; Stars; Interstellar medium; Envelope (radar); Circumstellar dust; Binary star; Carbon fibers; Carbon star","score_opus":0.018395873876054805,"score_gpt":0.2116022024795354,"score_spread":0.19320632860348058,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078020380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996137,0.000077111355,0.000028117332,0.0000034129362,5.410359e-7,7.10165e-7,0.000021725464,0.00000232449,0.00025234002],"genre_scores_gemma":[0.9997758,0.000021109221,0.0000279592,0.0000019226459,0.0000023011169,6.597213e-7,0.00007622834,9.999416e-7,0.00009308416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999453,0.000006271042,0.000005555073,0.000018392779,0.0000140343445,0.000010398591],"domain_scores_gemma":[0.9997198,0.000035725257,0.00016003563,0.000019613875,0.000019411358,0.000045330453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001104098,0.00015234851,0.00019190225,0.0004598386,0.00024011687,0.00061293744,0.00012959634,0.00020576027,0.00050489267],"category_scores_gemma":[0.0005951211,0.00014948376,0.000081165075,0.0003362082,0.00022744767,0.00018890729,0.00025343095,0.00018565824,0.00019620846],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045190024,0.000075207674,0.92724144,0.000033828484,0.00003671795,0.0010166087,0.00021840801,0.0004182179,0.066202074,0.0002828931,0.000090445916,0.0039322646],"study_design_scores_gemma":[0.0000112508515,0.00009386074,0.99502903,0.0000029907583,0.000009621069,0.0014044754,0.000092299524,0.0005325363,0.0024463576,0.00012509138,0.0002487298,0.0000038011422],"about_ca_topic_score_codex":0.0005757962,"about_ca_topic_score_gemma":0.00049587875,"teacher_disagreement_score":0.00061293744,"about_ca_system_score_codex":0.00013004546,"about_ca_system_score_gemma":0.000029816358,"threshold_uncertainty_score":0.0016890168},"labels":[],"label_agreement":null},{"id":"W2078042492","doi":"10.1088/0004-637x/701/2/1627","title":"TWO RAPIDLY VARIABLE GALACTIC X-RAY TRANSIENTS OBSERVED WITH<i>CHANDRA</i>,<i>XMM-NEWTON</i>, AND<i>SUZAKU</i>","year":2009,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Sky; Stars; Binary number; X-ray; Observatory; Star formation; Astronomy; Optics","score_opus":0.014430315661892769,"score_gpt":0.22105805858005956,"score_spread":0.2066277429181668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078042492","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978928,0.00011761906,0.00032976165,0.00003210259,0.000011625978,0.000012161771,0.00031325416,0.00004854943,0.0012421076],"genre_scores_gemma":[0.99443984,0.00009478752,0.0019381323,0.00006474176,0.00002175301,0.000014783634,0.0024265859,0.000018508292,0.0009808068],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998926,0.0000048021207,0.000006508531,0.00003137001,0.00002757301,0.000037074853],"domain_scores_gemma":[0.99955267,0.000041691474,0.00012683118,0.000052034735,0.00005020192,0.00017660159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018164849,0.00027552305,0.00021661799,0.0009576525,0.00065042434,0.0006591144,0.0003522124,0.00038592395,0.0012874857],"category_scores_gemma":[0.0003225475,0.00023559744,0.00024401912,0.00058073096,0.00021476833,0.00037990336,0.00066873385,0.00039659656,0.00030534514],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089522585,0.0003265919,0.73968756,0.0001476486,0.00015015506,0.004831427,0.0014170955,0.00057905697,0.2251981,0.0009283618,0.0016030851,0.024235789],"study_design_scores_gemma":[0.00002196836,0.00021449983,0.979039,0.000012486589,0.000055038432,0.0016830962,0.00019932583,0.00066006265,0.013219741,0.00007636507,0.0047960556,0.000022362266],"about_ca_topic_score_codex":0.0027911908,"about_ca_topic_score_gemma":0.008607467,"teacher_disagreement_score":0.0027911908,"about_ca_system_score_codex":0.00035343555,"about_ca_system_score_gemma":0.00021232078,"threshold_uncertainty_score":0.005549848},"labels":[],"label_agreement":null},{"id":"W2078112089","doi":"10.1088/0004-637x/788/1/81","title":"BANYAN. III. RADIAL VELOCITY, ROTATION, AND X-RAY EMISSION OF LOW-MASS STAR CANDIDATES IN NEARBY YOUNG KINEMATIC GROUPS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Stars; Physics; Astrophysics; Proper motion; Parallax; Radial velocity; Photometry (optics); Astrometry; Low Mass; Astronomy","score_opus":0.005092069984549982,"score_gpt":0.2072260971807674,"score_spread":0.20213402719621743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078112089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9934655,0.00017814919,0.00048998365,0.000031838263,0.0000071974414,0.000012719132,0.0008449901,0.000023935025,0.0049456023],"genre_scores_gemma":[0.9907698,0.0001684848,0.0014792293,0.00002744779,0.000011281569,0.000025883312,0.004327514,0.000021230204,0.0031691159],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997825,0.000020030304,0.000012007443,0.00008107564,0.000046758858,0.0000576625],"domain_scores_gemma":[0.99970573,0.000023324534,0.00010443167,0.00003156664,0.00005493891,0.00007997057],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039815519,0.00022810788,0.00029281454,0.0019536316,0.0009006467,0.0012210063,0.00054431753,0.00016177933,0.0036315483],"category_scores_gemma":[0.0003399876,0.00012695378,0.0001547011,0.0013746682,0.0002757012,0.00026108275,0.00054568716,0.00020977085,0.001388801],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023435571,0.00009253072,0.95949,0.00004240836,0.000047154812,0.00030845634,0.0004797408,0.00019499735,0.011687881,0.00058833044,0.0008248479,0.0260093],"study_design_scores_gemma":[0.0000054334255,0.000016685133,0.9955177,0.000010564318,0.000011948277,0.00020591162,0.00026119183,0.00030310723,0.0011156532,0.00009200009,0.0024535896,0.0000062462527],"about_ca_topic_score_codex":0.023194082,"about_ca_topic_score_gemma":0.035900816,"teacher_disagreement_score":0.023194082,"about_ca_system_score_codex":0.00054376916,"about_ca_system_score_gemma":0.00046770216,"threshold_uncertainty_score":0.04611814},"labels":[],"label_agreement":null},{"id":"W2078121670","doi":"10.1088/0004-637x/698/2/2075","title":"<i>IRAS</i>-BASED WHOLE-SKY UPPER LIMIT ON DYSON SPHERES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"SPHERES; Black-body radiation; Luminosity; Limit (mathematics); Star (game theory); Infrared; Resolution (logic)","score_opus":0.012096076813969665,"score_gpt":0.26474199619329647,"score_spread":0.2526459193793268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078121670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5480671,0.008369714,0.12911499,0.0020119366,0.0006197526,0.00031157103,0.023822878,0.0067494474,0.2809326],"genre_scores_gemma":[0.92191625,0.0011195134,0.045439392,0.000743685,0.000333769,0.00015310131,0.022636965,0.0003736175,0.007283774],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99888366,0.000118081625,0.00008194719,0.00021715532,0.00042548383,0.0002737211],"domain_scores_gemma":[0.99537563,0.0014324954,0.00061741733,0.0008785804,0.0011644996,0.00053136045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019801483,0.0010234377,0.0006319631,0.0060827667,0.0012166776,0.0021857854,0.0010467706,0.0009271309,0.011345117],"category_scores_gemma":[0.0039939964,0.0003820591,0.0006807795,0.0019666606,0.00066861854,0.0011443404,0.0019842556,0.0007381672,0.0059837583],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028357634,0.00046648522,0.46286812,0.001371381,0.0004107318,0.0023048986,0.0010564829,0.009896001,0.14576477,0.07525411,0.099143855,0.19862738],"study_design_scores_gemma":[0.00008544504,0.00040151644,0.639805,0.0004362533,0.00021868724,0.0028514063,0.00065458094,0.02962098,0.08455927,0.031452347,0.20976761,0.00014699066],"about_ca_topic_score_codex":0.00285769,"about_ca_topic_score_gemma":0.0032300365,"teacher_disagreement_score":0.011345117,"about_ca_system_score_codex":0.0008010578,"about_ca_system_score_gemma":0.00029371373,"threshold_uncertainty_score":0.037953198},"labels":[],"label_agreement":null},{"id":"W2078442154","doi":"10.1088/0004-637x/732/2/124","title":"<i>AKARI</i>NEAR-INFRARED SPECTRAL OBSERVATIONS OF SHOCKED H<sub>2</sub>GAS OF THE SUPERNOVA REMNANT IC 443","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Supernova remnant; Spectral line; Emission spectrum; Population; Supernova; Spectral index; Thermal; Near-Earth supernova","score_opus":0.025576812540479974,"score_gpt":0.21550714246903538,"score_spread":0.1899303299285554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078442154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988023,0.00008948492,0.00025189557,0.0000071721906,0.0000020974949,0.000001939577,0.00015736067,0.000034212364,0.0006535818],"genre_scores_gemma":[0.9980326,0.00007772158,0.0008474704,0.00001541563,0.0000054540446,0.0000034902655,0.0006672804,0.000008839931,0.00034172685],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999763,0.0000016723958,0.0000013914336,0.0000066254643,0.0000070873457,0.00000693124],"domain_scores_gemma":[0.9999558,0.000004784782,0.000015062643,0.0000045913494,0.0000073539227,0.000012410579],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004935148,0.00013087271,0.000084397005,0.0004994796,0.000196464,0.00015749858,0.00013438977,0.00014065705,0.0010129161],"category_scores_gemma":[0.00006494593,0.00007495593,0.00015644277,0.0002920172,0.00008954048,0.00010813902,0.00019906768,0.0001616136,0.00016455486],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005093632,0.000064154316,0.20667891,0.00007459589,0.00010144432,0.00087728916,0.00022823272,0.0009155457,0.7786267,0.00017056729,0.0004943716,0.011258843],"study_design_scores_gemma":[0.0000046878254,0.00006495357,0.9736509,0.0000026420494,0.000021644513,0.0004756973,0.00006295697,0.00095102395,0.023906609,0.00004044985,0.00081040704,0.000008082751],"about_ca_topic_score_codex":0.0017338053,"about_ca_topic_score_gemma":0.0022653511,"teacher_disagreement_score":0.0017338053,"about_ca_system_score_codex":0.00009195206,"about_ca_system_score_gemma":0.000045181794,"threshold_uncertainty_score":0.0034473538},"labels":[],"label_agreement":null},{"id":"W2078473962","doi":"10.1086/423310","title":"Theoretical Modeling of Weakly Lensed Polarized Radio Sources","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Redshift; Quasar; Polarization (electrochemistry); Astrophysics; Galaxy; Radio galaxy","score_opus":0.008433683460366801,"score_gpt":0.21277381849234847,"score_spread":0.20434013503198167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078473962","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1928111,0.00039387334,0.7822444,0.0013961039,0.0000314257,0.00006328762,0.0003451002,0.00025412216,0.022460656],"genre_scores_gemma":[0.95686036,0.00067128334,0.034876592,0.0002163424,0.00017866684,0.00018737218,0.000403311,0.00008946117,0.006516585],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99938965,0.00018694553,0.000022607008,0.00010096281,0.00019796859,0.00010180661],"domain_scores_gemma":[0.99685127,0.0015614118,0.0007245426,0.00028346665,0.0003466495,0.00023267262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001647529,0.00074309326,0.0006593453,0.0017580981,0.00068307127,0.002286182,0.00250363,0.0012507502,0.0026383507],"category_scores_gemma":[0.0073293643,0.00047848717,0.0007133003,0.0009109383,0.001969042,0.0025076007,0.0016793286,0.00090197637,0.00059658947],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000038821887,0.000020662814,0.0043259664,0.0000345691,0.000026509724,0.00027496897,0.00021242241,0.20035593,0.0017063892,0.7868789,0.00052350806,0.00560137],"study_design_scores_gemma":[0.00001541807,0.000015704813,0.0008973672,0.000009075017,0.000011339803,0.00014719892,0.00003686721,0.75133276,0.00029792963,0.24645871,0.000757816,0.00001975427],"about_ca_topic_score_codex":0.002269323,"about_ca_topic_score_gemma":0.00090831524,"teacher_disagreement_score":0.0026383507,"about_ca_system_score_codex":0.0012056499,"about_ca_system_score_gemma":0.0005106248,"threshold_uncertainty_score":0.008826137},"labels":[],"label_agreement":null},{"id":"W2078495633","doi":"10.1088/0004-637x/796/2/105","title":"THE NORMA ARM REGION<i>CHANDRA</i>SURVEY CATALOG: X-RAY POPULATIONS IN THE SPIRAL ARMS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Spiral galaxy; Population; Stars; Spiral (railway); Spectral line; Conjunction (astronomy); Remainder","score_opus":0.03891549036206948,"score_gpt":0.2621334574491335,"score_spread":0.22321796708706404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078495633","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8836662,0.0012432184,0.0011159655,0.00019906962,0.000025065943,0.00016317324,0.098789975,0.0008008716,0.013996432],"genre_scores_gemma":[0.7438179,0.001926462,0.010231358,0.0003000197,0.0001690523,0.00034716472,0.23648003,0.00024894314,0.0064790654],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997181,0.00002615756,0.000033975888,0.000055897497,0.00009826177,0.00006752499],"domain_scores_gemma":[0.9983847,0.00009514204,0.0005276218,0.0002690345,0.00035597393,0.00036752707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004996146,0.00031214766,0.00024335786,0.0051661134,0.0004040412,0.0007335938,0.00047496182,0.00012096978,0.0039061364],"category_scores_gemma":[0.0012505596,0.0001587883,0.00023119301,0.003921564,0.00013670446,0.0004970322,0.0009239189,0.0001564465,0.0016066204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024085162,0.00006385233,0.8758948,0.0002063444,0.00010610339,0.00021117284,0.0007232036,0.00030860142,0.009651865,0.0009144622,0.045632925,0.06604586],"study_design_scores_gemma":[0.000017137927,0.000022611735,0.968531,0.000034757184,0.000021119815,0.00045802936,0.00013593007,0.00041288507,0.0006232428,0.00013227003,0.029599687,0.000011410748],"about_ca_topic_score_codex":0.015924554,"about_ca_topic_score_gemma":0.027966755,"teacher_disagreement_score":0.015924554,"about_ca_system_score_codex":0.00040873472,"about_ca_system_score_gemma":0.0006364577,"threshold_uncertainty_score":0.031663716},"labels":[],"label_agreement":null},{"id":"W2078495797","doi":"10.1088/0004-637x/765/2/133","title":"CONTINUUM VARIABILITY OF DEEPLY EMBEDDED PROTOSTARS AS A PROBE OF ENVELOPE STRUCTURE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"National Research Council Canada; Natural Sciences and Engineering Research Council of Canada; European Southern Observatory; Academia Sinica","keywords":"Physics; Astrophysics; Stars; Protostar; Accretion (finance); Spectral energy distribution; Wavelength; Envelope (radar); Amplitude; Astronomy; Photon; Star formation; Optics; Galaxy","score_opus":0.005477843386831414,"score_gpt":0.2243822005670971,"score_spread":0.21890435718026569,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078495797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99789643,0.00015349826,0.00073249824,0.000016572418,0.0000026046614,0.0000044033272,0.00012185551,0.000030478845,0.0010415954],"genre_scores_gemma":[0.99890304,0.000053944714,0.0006522535,0.000021579914,0.0000050861486,0.0000040447767,0.00013664403,0.0000057811917,0.00021759757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999304,0.000009132404,0.0000029557243,0.000026746187,0.000014793048,0.000015974687],"domain_scores_gemma":[0.99968517,0.00007032858,0.00010569023,0.000029304394,0.000027574311,0.00008196595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019942182,0.00013635946,0.00017571491,0.0004634011,0.00020432391,0.0005121849,0.00018121496,0.00036446966,0.00075024995],"category_scores_gemma":[0.00033059463,0.0001235395,0.00013034801,0.00037488854,0.0001343717,0.0002979349,0.00031662823,0.00039281466,0.00023854033],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004052116,0.00019032898,0.68719155,0.000049023754,0.00008266154,0.00029940042,0.00037135437,0.0007511132,0.29416114,0.0002885928,0.00016539634,0.016044334],"study_design_scores_gemma":[0.0000030699168,0.00012733294,0.99285406,0.0000047850713,0.000009977986,0.00029448868,0.00014112779,0.0009474849,0.0051285364,0.00016614445,0.00031953945,0.000003456917],"about_ca_topic_score_codex":0.00029069887,"about_ca_topic_score_gemma":0.00058837514,"teacher_disagreement_score":0.00075024995,"about_ca_system_score_codex":0.00011734132,"about_ca_system_score_gemma":0.00004817159,"threshold_uncertainty_score":0.0025098324},"labels":[],"label_agreement":null},{"id":"W2078590695","doi":"10.1086/587887","title":"The Evolutionary History of Galactic Bulges: Photometric and Spectroscopic Studies of Distant Spheroids in the GOODS Fields","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Bulge; Astrophysics; Physics; Star formation; Galaxy; Stellar mass; Redshift; Astronomy; Spiral galaxy; Galaxy formation and evolution; Context (archaeology); Luminosity; Disc; Surface brightness; Geography","score_opus":0.017159056264334123,"score_gpt":0.2383753107863089,"score_spread":0.2212162545219748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078590695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995902,0.000085700114,0.000058099475,0.000004916219,4.9477393e-7,0.0000012459534,0.000048903996,0.0000012366582,0.00020923921],"genre_scores_gemma":[0.99956423,0.00005533119,0.000092507704,0.000005876456,0.0000030817555,0.000001126298,0.00015326962,0.0000011805889,0.00012338694],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998292,0.000022670289,0.000011117762,0.000061483115,0.0000331349,0.00004239514],"domain_scores_gemma":[0.99888927,0.00017605169,0.00036998483,0.00012539946,0.00014926687,0.00029001335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003649684,0.0001783087,0.00024110243,0.0016787938,0.00047455786,0.0005245621,0.00021040686,0.00016862703,0.00064702844],"category_scores_gemma":[0.00090554747,0.0001141052,0.00015233849,0.00095472124,0.0006613705,0.0004838306,0.0008195654,0.00019420388,0.0002007816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052249343,0.0000134673555,0.99138707,0.000008047948,0.0000133997755,0.000046735124,0.0006664346,0.000056156863,0.004148402,0.000058884674,0.000017449373,0.0035316371],"study_design_scores_gemma":[6.186512e-7,0.000020556037,0.9994287,0.0000010074716,0.0000033582676,0.000049944385,0.00020170344,0.000034493336,0.00015490215,0.000014324284,0.0000893607,9.413784e-7],"about_ca_topic_score_codex":0.0065610507,"about_ca_topic_score_gemma":0.010478812,"teacher_disagreement_score":0.0065610507,"about_ca_system_score_codex":0.00037979076,"about_ca_system_score_gemma":0.00014177414,"threshold_uncertainty_score":0.013045728},"labels":[],"label_agreement":null},{"id":"W2078609142","doi":"10.1086/497563","title":"The Linear Theory Power Spectrum from the Lyα Forest in the Sloan Digital Sky Survey","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":390,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Spectral density; Physics; Cosmic microwave background; Amplitude; Gaussian; Degeneracy (biology); Redshift; Spectral slope; Astrophysics; Degenerate energy levels; Linear model; Computational physics; Statistical physics; Statistics; Spectral line; Galaxy; Optics; Mathematics; Quantum mechanics","score_opus":0.0066368865450148196,"score_gpt":0.20737496788986595,"score_spread":0.20073808134485113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078609142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9888504,0.00018495413,0.0029137677,0.00017843425,0.00000586253,0.000009023117,0.0034545648,0.00030340825,0.004099524],"genre_scores_gemma":[0.9948317,0.00006889098,0.0010284719,0.000037314472,0.000007210412,0.000008641725,0.0035961547,0.000048082093,0.00037339196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978644,0.00005440836,0.000007902352,0.000046987465,0.000050566778,0.000053750493],"domain_scores_gemma":[0.999511,0.000113980306,0.0001283013,0.0000863997,0.00009386455,0.000066440836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060451205,0.00032143106,0.00013326273,0.0011192838,0.00023478926,0.0005211696,0.00025753994,0.00020831743,0.0015715782],"category_scores_gemma":[0.0012290581,0.00014747858,0.00037012948,0.0012281517,0.0002754054,0.0003219825,0.00042261486,0.00021905512,0.000442162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021447902,0.000049463582,0.8429831,0.00015220637,0.00023557665,0.00043689547,0.00030508757,0.10900871,0.0070650894,0.0075556114,0.007890137,0.02410349],"study_design_scores_gemma":[0.000025413858,0.000024510035,0.8743063,0.000027233253,0.000028690763,0.00008198892,0.00011794756,0.117712796,0.0014027833,0.0026447172,0.0036017664,0.000025883413],"about_ca_topic_score_codex":0.031376235,"about_ca_topic_score_gemma":0.025064379,"teacher_disagreement_score":0.031376235,"about_ca_system_score_codex":0.00088488206,"about_ca_system_score_gemma":0.00033479976,"threshold_uncertainty_score":0.062387228},"labels":[],"label_agreement":null},{"id":"W2078687139","doi":"10.1088/0004-637x/735/1/46","title":"ON THE MODE OF DYNAMO ACTION IN A GLOBAL LARGE-EDDY SIMULATION OF SOLAR CONVECTION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":187,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Canadian Space Agency","funders":"","keywords":"Physics; Dynamo; Solar dynamo; Convection zone; Mechanics; Classical mechanics; Dynamo theory; Interplanetary magnetic field; Magnetohydrodynamics; Convection; Magnetic field; Geophysics; Turbulence; Computational physics; Solar wind; Quantum mechanics","score_opus":0.015554755371139891,"score_gpt":0.2676714961084619,"score_spread":0.25211674073732204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078687139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903561,0.000060256483,0.0063820677,0.00021613215,0.000017298562,0.00002523391,0.00007464684,0.00010693799,0.0027613423],"genre_scores_gemma":[0.9968811,0.000031053514,0.0026217878,0.000032952772,0.0000070326973,0.000015841355,0.000048755555,0.000032883174,0.00032858833],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998865,0.00005320469,0.0000047591893,0.00001377548,0.000020086969,0.000021545176],"domain_scores_gemma":[0.9994579,0.00032775613,0.000061767474,0.000034173136,0.0000401035,0.00007834897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061215454,0.00038661438,0.00044826453,0.00031437862,0.00045461138,0.0007556047,0.0005548278,0.0007005839,0.0006820256],"category_scores_gemma":[0.0019421773,0.00019506276,0.00033219453,0.00031594135,0.0008203256,0.00061336375,0.00068540906,0.0005478225,0.00007032043],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016526671,0.00011688136,0.009137172,0.000023426152,0.00003402749,0.0001579245,0.00013911823,0.9827571,0.00277555,0.0023679496,0.0001912491,0.0021343264],"study_design_scores_gemma":[0.0000151151735,0.000019394167,0.00065891386,0.000001632216,0.0000019403149,0.000004318766,0.000024065754,0.9987326,0.00020239971,0.00027119898,0.000065377906,0.000002987425],"about_ca_topic_score_codex":0.007567573,"about_ca_topic_score_gemma":0.0057989843,"teacher_disagreement_score":0.007567573,"about_ca_system_score_codex":0.00044983273,"about_ca_system_score_gemma":0.0005283366,"threshold_uncertainty_score":0.015047073},"labels":[],"label_agreement":null},{"id":"W2078883760","doi":"10.1086/524134","title":"The Ratio of Helium‐ to Hydrogen‐Atmosphere White Dwarfs: Direct Evidence for Convective Mixing","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Atmosphere (unit); White dwarf; Effective temperature; Helium; Convection; Hydrogen; Convective mixing; Astrophysics; Physics; Stars; Mixing ratio; Blue dwarf; Atmospheric sciences; Thermodynamics; Atomic physics","score_opus":0.025177638785925417,"score_gpt":0.2584171077573343,"score_spread":0.23323946897140888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078883760","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992725,0.000060141854,0.00023433003,0.0000044212866,8.7976224e-7,0.0000011548275,0.00009189728,0.000012413377,0.00032228307],"genre_scores_gemma":[0.9995721,0.000023392473,0.00013531018,0.0000034271516,0.0000020692835,0.0000010083103,0.000164355,0.0000031441182,0.00009517583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998292,0.000019913567,0.00001454198,0.00006928837,0.000036713875,0.0000303052],"domain_scores_gemma":[0.9993893,0.00011129338,0.00020557061,0.00006288687,0.00007963357,0.00015132925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003071753,0.00019393225,0.00018424778,0.001137157,0.00023293853,0.0005480533,0.00022262384,0.00021110696,0.0007264394],"category_scores_gemma":[0.0010100357,0.00016474939,0.00013229101,0.00035659733,0.00026863263,0.00037646986,0.0003474887,0.00014480617,0.00031952848],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021065712,0.000019903371,0.94049764,0.000015323154,0.000052425552,0.00007105519,0.0001558856,0.00015885879,0.054270633,0.0001844292,0.000052534255,0.004310673],"study_design_scores_gemma":[0.0000043461914,0.00006370889,0.9911075,0.0000015994356,0.000012886823,0.0003558217,0.000057996374,0.0005715228,0.0075087757,0.00012944215,0.00018295889,0.0000034177208],"about_ca_topic_score_codex":0.0008075613,"about_ca_topic_score_gemma":0.000994846,"teacher_disagreement_score":0.001137157,"about_ca_system_score_codex":0.00014759142,"about_ca_system_score_gemma":0.000065365326,"threshold_uncertainty_score":0.002430141},"labels":[],"label_agreement":null},{"id":"W2078923655","doi":"10.1086/382067","title":"Tracing the Magnetic Field in Orion A","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Polarization (electrochemistry); Magnetic field; Protein filament; Polarimetry; Perpendicular; Orientation (vector space); Position angle; Sky; Astrophysics; Optics; Geometry; Materials science; Galaxy","score_opus":0.0076610537953933,"score_gpt":0.22871696303537026,"score_spread":0.22105590923997695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078923655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959772,0.00008504562,0.00046223047,0.000046481753,0.0000052419346,0.0000090404055,0.0004642363,0.000072158895,0.0028783598],"genre_scores_gemma":[0.9970847,0.00006630344,0.0016596654,0.00001830612,0.000009452273,0.000006765286,0.00067507784,0.000017611374,0.00046196708],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999088,0.000010582266,0.0000028772756,0.000039033457,0.000019835126,0.000018869949],"domain_scores_gemma":[0.99973637,0.000023986804,0.00008237169,0.000021717608,0.000056503624,0.00007913317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001675324,0.00020919582,0.00016278715,0.0015200662,0.0004862457,0.0005351046,0.0002949155,0.0002433145,0.00080921355],"category_scores_gemma":[0.00040995557,0.00017724419,0.00013340959,0.00089891785,0.0002262628,0.00021810892,0.0005811154,0.0002513389,0.00023886123],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031737823,0.00013083676,0.8550687,0.00008812728,0.000088662164,0.000857882,0.002101271,0.0043130126,0.088631175,0.0009757634,0.0014221091,0.04600505],"study_design_scores_gemma":[0.000012930454,0.000057782294,0.9884525,0.000019432953,0.000013671565,0.000118699936,0.0003531585,0.0051037846,0.0024311335,0.00022541579,0.0031993696,0.000012041021],"about_ca_topic_score_codex":0.014275363,"about_ca_topic_score_gemma":0.018191034,"teacher_disagreement_score":0.014275363,"about_ca_system_score_codex":0.00045652842,"about_ca_system_score_gemma":0.00030350537,"threshold_uncertainty_score":0.028384566},"labels":[],"label_agreement":null},{"id":"W2078965538","doi":"10.1088/0004-637x/762/1/55","title":"<i>MOST</i>SPACE TELESCOPE PHOTOMETRY OF THE 2010 JANUARY TRANSIT OF EXTRASOLAR PLANET HD80606b","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Transit (satellite); Exoplanet; Physics; Photometry (optics); Spitzer Space Telescope; Planet; Stars; Astronomy; Limiting; Limiting magnitude; Telescope; Astrophysics","score_opus":0.009038184290264328,"score_gpt":0.21266535163801484,"score_spread":0.20362716734775052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2078965538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7179685,0.00070723647,0.0014828852,0.00074420363,0.00018134354,0.00010977455,0.20214255,0.0014864412,0.075177036],"genre_scores_gemma":[0.846266,0.00034900027,0.004774747,0.0003805613,0.00013202806,0.000042255324,0.13530561,0.00018876251,0.012560967],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998877,0.000003073855,0.0000052605387,0.000020586318,0.00003833927,0.000045020388],"domain_scores_gemma":[0.9996344,0.000010774449,0.00009373756,0.000042969466,0.000101267324,0.00011680111],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011094297,0.00023430175,0.00017430069,0.0029490902,0.0007771168,0.00046086195,0.00036440347,0.0002666075,0.008422156],"category_scores_gemma":[0.00029336696,0.00010387461,0.00017203794,0.0015370811,0.00018733279,0.00020366258,0.0005694439,0.00023028815,0.0020636567],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043480992,0.00025428113,0.6372101,0.00035783323,0.00013393744,0.00061902945,0.00078745914,0.0017676357,0.081267476,0.0015790142,0.20128047,0.07430798],"study_design_scores_gemma":[0.000012663352,0.000031282136,0.94403464,0.000021508016,0.000017295715,0.00024765744,0.000091453505,0.0005289978,0.0036150387,0.00012857259,0.051257137,0.000013733399],"about_ca_topic_score_codex":0.16819154,"about_ca_topic_score_gemma":0.49467024,"teacher_disagreement_score":0.16819154,"about_ca_system_score_codex":0.00083575584,"about_ca_system_score_gemma":0.00061094045,"threshold_uncertainty_score":0.33442515},"labels":[],"label_agreement":null},{"id":"W2079116441","doi":"10.1088/0004-637x/777/2/123","title":"ON THE CLUSTER PHYSICS OF SUNYAEV-ZEL'DOVICH AND X-RAY SURVEYS. III. MEASUREMENT BIASES AND COSMOLOGICAL EVOLUTION OF GAS AND STELLAR MASS FRACTIONS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Virial theorem; Sunyaev–Zel'dovich effect; Hydrostatic equilibrium; Galaxy cluster; Baryon; Cosmic variance; Dark matter; Cluster (spacecraft); RADIUS; Radiative cooling; Galaxy; Astronomy; Redshift","score_opus":0.02226846937591741,"score_gpt":0.21787289031698243,"score_spread":0.195604420941065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079116441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9764805,0.0016137459,0.01033812,0.0008181874,0.00003924188,0.000026949952,0.0014344429,0.00015899286,0.009089905],"genre_scores_gemma":[0.9958709,0.00037104654,0.0021120084,0.00009631299,0.00001891243,0.000014621851,0.0006288933,0.000055612916,0.00083178084],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997185,0.000095880365,0.0000096347885,0.00006821414,0.000056791203,0.00005094359],"domain_scores_gemma":[0.99935776,0.0002261393,0.00017338272,0.00010699958,0.000076400414,0.00005938302],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010024083,0.00028035877,0.0003286817,0.00072457304,0.00040775596,0.0008330696,0.0006112914,0.00037882925,0.001297497],"category_scores_gemma":[0.0028415583,0.00027491324,0.00036177193,0.00079488417,0.00061410485,0.0007548385,0.0008897921,0.00035743375,0.00021285935],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017495471,0.000032507298,0.7053155,0.0001267331,0.00045601488,0.00019995858,0.0005661342,0.19324689,0.0028416875,0.069440894,0.0043047396,0.02329404],"study_design_scores_gemma":[0.000043560078,0.00004171348,0.74346304,0.00007717178,0.000059419144,0.000085212516,0.00023258544,0.22392017,0.0018331122,0.020829996,0.00935904,0.00005511306],"about_ca_topic_score_codex":0.03034583,"about_ca_topic_score_gemma":0.023362175,"teacher_disagreement_score":0.03034583,"about_ca_system_score_codex":0.0012230526,"about_ca_system_score_gemma":0.00059665483,"threshold_uncertainty_score":0.060338378},"labels":[],"label_agreement":null},{"id":"W2079125871","doi":"10.1086/379644","title":"Matching Stellar Models to Oscillation Data","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Oscillation (cell signaling); Astrophysics; Luminosity; Mode (computer interface); Data set; Measure (data warehouse); Star (game theory); Stellar mass; Matching (statistics); Stars; Star formation; Statistics; Data mining; Galaxy","score_opus":0.035645688475356666,"score_gpt":0.2557876208598186,"score_spread":0.22014193238446195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079125871","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08071096,0.000118662414,0.9092101,0.00009531937,0.00007120671,0.00012633293,0.0022679288,0.00470095,0.0026985798],"genre_scores_gemma":[0.43633235,0.00013925857,0.54962116,0.00012615215,0.000072740084,0.00027698887,0.010487852,0.0013145709,0.0016289363],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9982187,0.0004855827,0.00012516335,0.00059911737,0.00044714293,0.00012420697],"domain_scores_gemma":[0.99516857,0.0011761879,0.00042057643,0.0021158333,0.00096402835,0.00015488412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002495696,0.00081674237,0.0008789724,0.0029970377,0.00081907073,0.0015837958,0.0017469758,0.0011461322,0.0038816142],"category_scores_gemma":[0.017807541,0.0006623176,0.0014201346,0.002244717,0.00034014822,0.0017527171,0.001930088,0.0011516431,0.0032603878],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048339707,0.00057405536,0.10676297,0.0002583855,0.00076807564,0.00031761508,0.0006690012,0.36026454,0.02271954,0.017386729,0.011297295,0.4784984],"study_design_scores_gemma":[0.00006951006,0.00008923949,0.011443454,0.00003317982,0.000090826004,0.00020599649,0.00011258809,0.9420089,0.0112052625,0.023130735,0.011522361,0.00008784825],"about_ca_topic_score_codex":0.004046167,"about_ca_topic_score_gemma":0.0032423937,"teacher_disagreement_score":0.004046167,"about_ca_system_score_codex":0.00069827825,"about_ca_system_score_gemma":0.0008479701,"threshold_uncertainty_score":0.013198614},"labels":[],"label_agreement":null},{"id":"W2079141294","doi":"10.1086/321733","title":"Inferring Initial Spin Periods for Neutron Stars in Composite Remnants","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Supernova; Pulsar; Neutron star; Astrophysics; RADIUS; Luminosity; Pulsar wind nebula; Astronomy; Supernova remnant; Magnetar; Spin (aerodynamics); Nebula; Stars","score_opus":0.023784512409846373,"score_gpt":0.36667006786943246,"score_spread":0.3428855554595861,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079141294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96073645,0.00022938827,0.03698195,0.000017651735,0.000008947393,0.000013831692,0.00026712095,0.00017520995,0.0015693576],"genre_scores_gemma":[0.98734283,0.00009791762,0.011900742,0.0000033823046,0.000007948451,0.0000093958015,0.0004455757,0.000015285545,0.00017687387],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999392,0.000012777242,0.000006138403,0.000018539786,0.000013190229,0.000010146755],"domain_scores_gemma":[0.99930453,0.00019810036,0.00019835368,0.00010603558,0.00009542306,0.000097546865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044111416,0.0002151557,0.00017914527,0.001646204,0.00027030488,0.00041551716,0.00021931448,0.00018807157,0.00055411825],"category_scores_gemma":[0.0024764438,0.00023242341,0.000227104,0.00040092244,0.00018668854,0.00042616503,0.0004898356,0.00022450648,0.00027740924],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011580127,0.000070759546,0.8295811,0.00010311991,0.00013914744,0.0007707108,0.0006308261,0.029617539,0.04403349,0.00413469,0.0005366311,0.08922398],"study_design_scores_gemma":[0.000080938335,0.00035158946,0.63397175,0.000045654902,0.00013417826,0.0018264112,0.00031254976,0.31108597,0.039107703,0.008569288,0.0044244346,0.000089495516],"about_ca_topic_score_codex":0.0015005692,"about_ca_topic_score_gemma":0.0018460373,"teacher_disagreement_score":0.001646204,"about_ca_system_score_codex":0.00016955522,"about_ca_system_score_gemma":0.00017820162,"threshold_uncertainty_score":0.0029836297},"labels":[],"label_agreement":null},{"id":"W2079304679","doi":"10.1088/0004-637x/788/2/125","title":"AN ALMA SURVEY OF SUBMILLIMETER GALAXIES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH: THE REDSHIFT DISTRIBUTION AND EVOLUTION OF SUBMILLIMETER GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":333,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Key Programme; National Institutes of Natural Sciences; Danmarks Grundforskningsfond; National Astronomical Observatory of Japan; National Science Council; Leverhulme Trust; National Aeronautics and Space Administration; National Radio Astronomy Observatory; European Southern Observatory; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Astronomy; Photometric redshift; Photometry (optics); Star formation; Stellar mass; Galaxy formation and evolution; Chandra Deep Field South; Stars","score_opus":0.00921283004517596,"score_gpt":0.21812172676835784,"score_spread":0.20890889672318189,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079304679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99800366,0.00013514825,0.00033995244,0.000026617117,0.000002352022,0.0000062611875,0.0010020867,0.00003868165,0.0004452583],"genre_scores_gemma":[0.99636555,0.000119101336,0.0012577276,0.000028084993,0.00001335052,0.000010738007,0.0019526834,0.000011638047,0.0002411233],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982256,0.000026046728,0.000007585598,0.000050470033,0.000042450643,0.000050908868],"domain_scores_gemma":[0.99925333,0.000101613194,0.0002734156,0.0001089693,0.000083005165,0.00017959766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037267356,0.00030907235,0.00025593687,0.0016913457,0.00026259286,0.00043282143,0.00031044887,0.0001593138,0.0008170222],"category_scores_gemma":[0.0007710996,0.00019582159,0.0003262152,0.0010777864,0.00016799278,0.00033714547,0.00057915004,0.00023738391,0.00031655672],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007298198,0.000031029293,0.9805977,0.000025570998,0.00006477541,0.00006790529,0.00017997032,0.00035217378,0.0064547374,0.00024442977,0.00064310414,0.011265735],"study_design_scores_gemma":[0.0000036371516,0.000016712544,0.99816257,0.000003208866,0.000011698018,0.000083976294,0.000035698606,0.00057301903,0.00035031512,0.000047962287,0.0007077835,0.0000034431723],"about_ca_topic_score_codex":0.010416868,"about_ca_topic_score_gemma":0.016264958,"teacher_disagreement_score":0.010416868,"about_ca_system_score_codex":0.00031978142,"about_ca_system_score_gemma":0.00028175404,"threshold_uncertainty_score":0.020712435},"labels":[],"label_agreement":null},{"id":"W2079349148","doi":"10.1088/0004-637x/708/2/1585","title":"ON THE ROLE OF DISKS IN THE FORMATION OF STELLAR SYSTEMS: A NUMERICAL PARAMETER STUDY OF RAPID ACCRETION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":328,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Dimensionless quantity; Astrophysics; Gravitation; Isothermal process; Binary number; Star formation; Spiral galaxy; Accretion disc; Mechanics; Astronomy; Stars; Thermodynamics","score_opus":0.013002084237553531,"score_gpt":0.2435114009731409,"score_spread":0.23050931673558736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079349148","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960891,0.00009228108,0.0025015753,0.000078871395,0.0000036114966,0.000011165133,0.00003859209,0.000023371731,0.0011615483],"genre_scores_gemma":[0.9971687,0.00005872313,0.0025606307,0.000014690152,0.000003079,0.000012730896,0.000033235636,0.000012655203,0.00013546458],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998939,0.00004145051,0.000006015283,0.000018192059,0.000020129208,0.000020314712],"domain_scores_gemma":[0.99754745,0.0018031561,0.00030758136,0.00014646322,0.00009263874,0.00010264114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006320354,0.00041783685,0.00044814788,0.0006030279,0.00061822153,0.0008755862,0.0005715341,0.0006672251,0.000551524],"category_scores_gemma":[0.005126822,0.00025038887,0.00032772112,0.00038756366,0.0013211532,0.00085450435,0.00060182216,0.00048546464,0.00006278655],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021399422,0.00019305001,0.02035773,0.00006181605,0.00004561874,0.00031618756,0.00031413205,0.9593581,0.011092647,0.0046642744,0.00016653542,0.003215939],"study_design_scores_gemma":[0.000038420476,0.000087277185,0.0026802004,0.000005003652,0.000012352546,0.000051659743,0.000071710754,0.99389124,0.0015688161,0.0014743736,0.00010873772,0.000010191051],"about_ca_topic_score_codex":0.0032897072,"about_ca_topic_score_gemma":0.0021536446,"teacher_disagreement_score":0.0032897072,"about_ca_system_score_codex":0.000546062,"about_ca_system_score_gemma":0.00036151215,"threshold_uncertainty_score":0.0065410733},"labels":[],"label_agreement":null},{"id":"W2079484075","doi":"10.1086/522294","title":"Formaldehyde as a Tracer of Extragalactic Molecular Gas. I. Para‐H<sub>2</sub>CO Emission from M82","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Mean kinetic temperature; Galaxy; Astrophysics; Line (geometry); TRACER; Formaldehyde; Physics; Kinetic energy; Paraformaldehyde; Emission spectrum; Analytical Chemistry (journal); Chemistry; Spectral line; Astronomy","score_opus":0.008608289830733336,"score_gpt":0.2534657509147352,"score_spread":0.2448574610840019,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079484075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9845664,0.004000251,0.0053659636,0.0001029763,0.000012120833,0.000011643914,0.00031937083,0.00010233027,0.0055189724],"genre_scores_gemma":[0.99668425,0.0005173067,0.0021944342,0.00001985055,0.000009526997,0.000004285203,0.00012540241,0.0000071779114,0.00043780534],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994695,0.000008007088,0.0000015417038,0.000015251809,0.000015464417,0.000012737277],"domain_scores_gemma":[0.9999119,0.000022470515,0.000031703043,0.000011982604,0.000008997282,0.000012994893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000094603514,0.00021356843,0.0001071902,0.00044935054,0.00013589334,0.00028909085,0.00030924127,0.00032616235,0.00047998692],"category_scores_gemma":[0.00015004157,0.00011124839,0.00008619696,0.0004374814,0.00022554857,0.00026135545,0.00023494645,0.0001512799,0.00012641153],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002890384,0.00008599858,0.28383082,0.00018494787,0.00009060394,0.0006477006,0.00013867738,0.0056409524,0.674339,0.004015724,0.00044253442,0.030293876],"study_design_scores_gemma":[0.000031990305,0.0004860312,0.693715,0.000039879604,0.00010493899,0.00096805935,0.00023840937,0.028554335,0.2658789,0.0020389636,0.007913848,0.000029709468],"about_ca_topic_score_codex":0.0022975598,"about_ca_topic_score_gemma":0.0046742046,"teacher_disagreement_score":0.0022975598,"about_ca_system_score_codex":0.00037354397,"about_ca_system_score_gemma":0.000058488262,"threshold_uncertainty_score":0.004568398},"labels":[],"label_agreement":null},{"id":"W2079547342","doi":"10.1086/374970","title":"Discovery of Highly Dynamic Matter Enhancements along the Polar Axis and Equatorial Plane in the Luminous Blue Variable Binary HD 5980","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Luminous blue variable; Astrophysics; Polar; Polarimetry; Eclipse; Neutron star; Small Magellanic Cloud; Orbital inclination; Astronomy; Orbital plane; Light curve; Binary number; Stars; Optics; Scattering","score_opus":0.00582775465231634,"score_gpt":0.208811186378103,"score_spread":0.20298343172578667,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079547342","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99931765,0.00006205648,0.0001016363,0.000012171647,0.000001920107,0.0000013972821,0.00004814673,0.000004748741,0.00045027392],"genre_scores_gemma":[0.9997584,0.000018561093,0.000079104284,0.000005921245,0.0000046868786,0.0000010966287,0.00006417586,0.0000014953387,0.000066655055],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999515,0.000004289957,0.0000026492671,0.000018169507,0.000011775941,0.000011581878],"domain_scores_gemma":[0.99984384,0.000020393298,0.000079572295,0.000012942893,0.000012747653,0.000030445388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000083538805,0.00008908976,0.00013472092,0.0005383221,0.00027254721,0.0003958002,0.0001208191,0.00018216085,0.00041457036],"category_scores_gemma":[0.00028119422,0.00009581847,0.000060570885,0.00027142206,0.00026483208,0.00015541894,0.00039009535,0.00018380613,0.00014156717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026813298,0.000060713806,0.73698664,0.000034812812,0.000043215638,0.002380995,0.0006830857,0.00017462787,0.24539708,0.00045036606,0.00030359035,0.013216717],"study_design_scores_gemma":[0.000004133125,0.000034595178,0.99596184,0.0000021673393,0.000009009454,0.0008104674,0.00009636782,0.00021865389,0.002289754,0.00007528876,0.0004945744,0.0000031228858],"about_ca_topic_score_codex":0.0010492466,"about_ca_topic_score_gemma":0.0017003809,"teacher_disagreement_score":0.0010492466,"about_ca_system_score_codex":0.0001305484,"about_ca_system_score_gemma":0.00006844036,"threshold_uncertainty_score":0.0020862222},"labels":[],"label_agreement":null},{"id":"W2079557743","doi":"10.1086/346075","title":"Extraordinary Diffuse Light in Hickson Compact Group 90","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Elliptical galaxy; Surface brightness; Astronomy; Galaxy group; Intracluster medium; Lenticular galaxy; Galaxy; Peculiar galaxy; Luminosity; Population; Surface brightness fluctuation; Stellar population; Brightness; Spiral galaxy; Galaxy cluster; Star formation; Medicine","score_opus":0.007893924829670032,"score_gpt":0.2135213960438552,"score_spread":0.20562747121418518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079557743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99919266,0.00007191493,0.000041123127,0.000004973766,0.0000011330985,0.0000031287375,0.000037646663,0.0000048115808,0.0006425823],"genre_scores_gemma":[0.9995732,0.00002988182,0.00005988947,0.000006870151,0.0000026528148,0.0000014532428,0.00014754455,0.0000024406918,0.00017612588],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998678,0.000009444423,0.0000070067285,0.000022797392,0.00003569887,0.000057147154],"domain_scores_gemma":[0.99976164,0.000013568186,0.00008021137,0.000011343564,0.00002474602,0.000108494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014047154,0.00027119677,0.0002017553,0.0021018162,0.00032842424,0.000481835,0.00020568063,0.00020020694,0.0010422057],"category_scores_gemma":[0.00023468137,0.00010511496,0.00019012034,0.00059230305,0.00026631865,0.00015517829,0.00071484025,0.000183192,0.0002563821],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005882846,0.00013410667,0.9330167,0.000036757214,0.000061660976,0.002668261,0.001019424,0.0001308656,0.04757763,0.00027969456,0.00032776053,0.014158748],"study_design_scores_gemma":[0.000006755771,0.00012903148,0.99602145,0.000003971884,0.000013006253,0.0021075697,0.0002825759,0.00012759076,0.00076608825,0.000052633248,0.00048448477,0.000004816983],"about_ca_topic_score_codex":0.0057380376,"about_ca_topic_score_gemma":0.0048237983,"teacher_disagreement_score":0.0057380376,"about_ca_system_score_codex":0.00029428466,"about_ca_system_score_gemma":0.00007547091,"threshold_uncertainty_score":0.011409283},"labels":[],"label_agreement":null},{"id":"W2079587369","doi":"10.1086/500421","title":"Spectral Variability of Quasars in the Sloan Digital Sky Survey. II. The C<scp>iv</scp>Line","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Quasar; Astrophysics; Physics; Redshift; Blueshift; Sky; Equivalent width; Line (geometry); Flux (metallurgy); Skewness; Ionization; Absolute magnitude; Astronomy; Spectral line; Emission spectrum; Optics; Galaxy; Chemistry; Geometry","score_opus":0.007805731899365979,"score_gpt":0.20942540242332205,"score_spread":0.20161967052395607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079587369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990103,0.00006250089,0.000049981787,0.000010303225,0.000001210804,0.000002330014,0.000626098,0.0000072446082,0.00022999757],"genre_scores_gemma":[0.99802065,0.000041252766,0.000092297225,0.000009241581,0.000003479585,0.000004316634,0.0017139766,0.0000022440495,0.00011250426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980766,0.000026596303,0.00002169926,0.000040776038,0.00005213385,0.000051244697],"domain_scores_gemma":[0.99873894,0.00015076579,0.0006834481,0.00007607632,0.00015385686,0.00019706444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003414036,0.00017528117,0.00015700032,0.0017898525,0.00019362997,0.0005189538,0.00016924026,0.00017862505,0.00048501365],"category_scores_gemma":[0.00088931626,0.000101395766,0.00017785127,0.0012360122,0.00028490176,0.00025475054,0.0004743367,0.00014729884,0.00017237454],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027711236,0.000009128318,0.9970944,0.000006663934,0.000029409553,0.00003976961,0.000075325006,0.000076445045,0.0008888017,0.000017908362,0.000101971214,0.0016324219],"study_design_scores_gemma":[4.87572e-7,0.000006510241,0.99972814,7.3814573e-7,0.0000027933945,0.000031979685,0.00003376868,0.00005488662,0.00003968634,0.0000035249234,0.000096687036,7.4573927e-7],"about_ca_topic_score_codex":0.010437124,"about_ca_topic_score_gemma":0.015874425,"teacher_disagreement_score":0.010437124,"about_ca_system_score_codex":0.0003335671,"about_ca_system_score_gemma":0.00012013189,"threshold_uncertainty_score":0.020752788},"labels":[],"label_agreement":null},{"id":"W2079626706","doi":"10.1088/0004-637x/759/1/34","title":"ORTHO-TO-PARA RATIO STUDIES OF SHOCKED H<sub>2</sub>GAS IN THE TWO SUPERNOVA REMNANTS IC 443 AND HB 21","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Supernova; Astrophysics; Thermal equilibrium; Infrared; Atomic physics; Range (aeronautics); Thermodynamics; Materials science; Astronomy","score_opus":0.03060674743417664,"score_gpt":0.2957923515321385,"score_spread":0.2651856040979619,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079626706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99924684,0.00011343765,0.00015884908,0.000006022729,0.0000015744556,0.000003201397,0.000051628325,0.000017358092,0.0004011494],"genre_scores_gemma":[0.9993394,0.00005955899,0.00028105424,0.000013032292,0.0000043546893,0.000003942543,0.00017953418,0.000007286885,0.00011177444],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992514,0.0000054119905,0.0000046139016,0.000023181989,0.000017128279,0.000024443389],"domain_scores_gemma":[0.9998523,0.000018693978,0.0000659634,0.000011106978,0.000018648112,0.00003339342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000084513216,0.00023546089,0.00018910138,0.00085459475,0.0002515729,0.00022248147,0.00028460857,0.00024555624,0.0009628856],"category_scores_gemma":[0.00017083857,0.00017881113,0.00023890065,0.00041681703,0.00023569787,0.00022752467,0.00036450563,0.00022831351,0.000118216645],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006005235,0.000115623676,0.25309262,0.000092740884,0.0001766095,0.0016078254,0.00035291325,0.0011951735,0.7332604,0.00019813782,0.00014040417,0.009167065],"study_design_scores_gemma":[0.000012877748,0.00014531512,0.9645574,0.000003273284,0.00005208763,0.00054329925,0.00019416145,0.0016787136,0.032327835,0.0000609457,0.00041124446,0.000012744127],"about_ca_topic_score_codex":0.0016115544,"about_ca_topic_score_gemma":0.0016032044,"teacher_disagreement_score":0.0016115544,"about_ca_system_score_codex":0.00017081902,"about_ca_system_score_gemma":0.000071815535,"threshold_uncertainty_score":0.0032211542},"labels":[],"label_agreement":null},{"id":"W2079748759","doi":"10.1088/0004-637x/728/1/51","title":"INTERPRETING THE EVOLUTION OF THE SIZE-LUMINOSITY RELATION FOR DISK GALAXIES FROM REDSHIFT 1 TO THE PRESENT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; McMaster University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Stellar mass; Redshift; Halo; Galaxy formation and evolution; Stellar population; Tully–Fisher relation; Surface brightness fluctuation; Thick disk","score_opus":0.010259148345679089,"score_gpt":0.21056670153531573,"score_spread":0.20030755318963664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079748759","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980356,0.000060482547,0.0010889756,0.00003383167,0.0000015444361,0.0000039813244,0.00030107636,0.000038710084,0.00043572817],"genre_scores_gemma":[0.99824333,0.000032033517,0.0009873408,0.000008335301,0.0000019171173,0.0000036554666,0.00055544527,0.000010951314,0.00015699866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990106,0.000021753172,0.000004205129,0.000040380848,0.000016919057,0.000015751566],"domain_scores_gemma":[0.9992853,0.00029060934,0.00019694316,0.000082017206,0.000068358815,0.00007687702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046830665,0.00019426427,0.00016256704,0.0006710392,0.00018463768,0.0006065675,0.0004383547,0.0004428677,0.0008610574],"category_scores_gemma":[0.0022690573,0.00018776466,0.00032401425,0.00039324423,0.00022705548,0.0003513634,0.00031364904,0.00031663667,0.00015905638],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016926602,0.00008186294,0.7552149,0.00005886276,0.0001563958,0.00022767787,0.00035156758,0.20539065,0.023372613,0.0043943687,0.00055800553,0.010023843],"study_design_scores_gemma":[0.00004573148,0.00013028443,0.6425354,0.000012076979,0.00007956513,0.00024624786,0.00013414361,0.34459552,0.0072665927,0.0026213536,0.0023031512,0.000029861234],"about_ca_topic_score_codex":0.0054479134,"about_ca_topic_score_gemma":0.006017592,"teacher_disagreement_score":0.0054479134,"about_ca_system_score_codex":0.0006020846,"about_ca_system_score_gemma":0.000119097145,"threshold_uncertainty_score":0.010832429},"labels":[],"label_agreement":null},{"id":"W2079790915","doi":"10.1088/0004-637x/708/1/253","title":"MODELING THE SYSTEM PARAMETERS OF 2M 1533+3759: A NEW LONGER PERIOD LOW-MASS ECLIPSING sdB+dM BINARY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Subdwarf; Astrophysics; Physics; Light curve; Orbital period; Stars; Mass ratio; Contact binary; Astronomy; Binary star; White dwarf","score_opus":0.014737567789004022,"score_gpt":0.22422270032340924,"score_spread":0.2094851325344052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079790915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99482924,0.00005633282,0.0025161759,0.000050190636,0.0000045219026,0.000012329021,0.00043303563,0.00005484231,0.0020433886],"genre_scores_gemma":[0.997288,0.000026765207,0.0016628606,0.000015204669,0.0000043397818,0.000011625937,0.00046683202,0.000021229756,0.0005031742],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999962,0.000005612924,0.0000016254354,0.000014344836,0.0000069832913,0.000009359876],"domain_scores_gemma":[0.99992967,0.00001642302,0.000017640816,0.000007868077,0.000008984701,0.000019408802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008203839,0.00028527467,0.000298696,0.00021457633,0.000290043,0.000432203,0.00037063597,0.00044103674,0.0013159047],"category_scores_gemma":[0.00029606323,0.00012719685,0.00028656184,0.00025457595,0.00016942142,0.00023079215,0.0002321333,0.0002007703,0.00032872212],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042058213,0.00020392599,0.29682627,0.00015549612,0.0001176151,0.0010497941,0.0004648029,0.6344037,0.0408214,0.0046691787,0.0026550626,0.01821218],"study_design_scores_gemma":[0.00006295107,0.0000837005,0.09392812,0.00001085663,0.00003554345,0.000284666,0.00013887398,0.897788,0.0025100803,0.0013232972,0.0038062634,0.000027622957],"about_ca_topic_score_codex":0.024150798,"about_ca_topic_score_gemma":0.02052999,"teacher_disagreement_score":0.024150798,"about_ca_system_score_codex":0.0012561859,"about_ca_system_score_gemma":0.0003342276,"threshold_uncertainty_score":0.048020422},"labels":[],"label_agreement":null},{"id":"W2079810189","doi":"10.1086/432536","title":"A Coherent Timing Solution for the Nearby Isolated Neutron Star RX J0720.4-3125","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Neutron star; Pulsar; Measure (data warehouse); Magnetic field; Phase (matter); Dipole; Star (game theory)","score_opus":0.021887783795777594,"score_gpt":0.3242638518158464,"score_spread":0.3023760680200688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079810189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83114624,0.00022581412,0.16115619,0.00026813048,0.00005705866,0.000040949923,0.0008174905,0.00050931645,0.005778785],"genre_scores_gemma":[0.880116,0.00013111136,0.11484246,0.00007181549,0.000052411615,0.000052243493,0.001895901,0.00012583977,0.0027121566],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99994934,0.000004997157,0.0000039988654,0.000017291408,0.000016431992,0.000007848957],"domain_scores_gemma":[0.9998006,0.000029115503,0.00007482784,0.000015630068,0.000052916253,0.00002684677],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015374745,0.0002800219,0.0001857032,0.00039518243,0.00021791956,0.00040221462,0.00037613662,0.00036715073,0.0021414969],"category_scores_gemma":[0.0010356264,0.00018435164,0.0002261321,0.00038635317,0.00010253091,0.00025910488,0.00033002024,0.00033498876,0.00036865642],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039727814,0.00020499802,0.0637285,0.00020978927,0.0001552502,0.0010725656,0.00034269306,0.59647226,0.13061866,0.02950069,0.0035702032,0.17372711],"study_design_scores_gemma":[0.00021441489,0.00023159028,0.04771514,0.000023300001,0.00006896988,0.00027976284,0.0001233766,0.92879087,0.011356857,0.006356549,0.0047881664,0.0000510103],"about_ca_topic_score_codex":0.004114956,"about_ca_topic_score_gemma":0.008103839,"teacher_disagreement_score":0.004114956,"about_ca_system_score_codex":0.0002971573,"about_ca_system_score_gemma":0.0006763323,"threshold_uncertainty_score":0.008181989},"labels":[],"label_agreement":null},{"id":"W2079814498","doi":"10.1086/519239","title":"First Constraints on Source Counts at 350 μm","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Source counts; Physics; Galaxy; Redshift; Spurious relationship; Astrophysics; Angular resolution (graph drawing); Field of view; Sensitivity (control systems); Population; Astronomy; Optics; Statistics; Mathematics","score_opus":0.007273470117774231,"score_gpt":0.21060037444384216,"score_spread":0.20332690432606793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079814498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8546645,0.001609129,0.07673461,0.0010188895,0.00007094003,0.00008568793,0.0063506663,0.0012509241,0.058214776],"genre_scores_gemma":[0.96474266,0.00030618487,0.028148007,0.0004898656,0.00008205125,0.00008022839,0.0033608223,0.00010584312,0.002684332],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991572,0.00013385712,0.00007042455,0.00018949911,0.00029506153,0.00015397694],"domain_scores_gemma":[0.9946861,0.0025836213,0.00077858614,0.0008817246,0.000706287,0.00036364535],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015121037,0.0004884106,0.0006146717,0.0012258101,0.0005727952,0.0014429367,0.00072710984,0.00060422375,0.00969342],"category_scores_gemma":[0.007595701,0.0004651244,0.00032745503,0.0007937828,0.00041278967,0.0012979024,0.0012072824,0.00063560274,0.0016526923],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008386021,0.00018769344,0.67645407,0.00044077451,0.0001486272,0.00057358755,0.0016370639,0.009582128,0.11164767,0.077027254,0.0148216,0.10664097],"study_design_scores_gemma":[0.00006179178,0.00027997128,0.8667676,0.00018103322,0.000091486574,0.0015108254,0.0004726713,0.02587865,0.031692173,0.039206,0.03375756,0.00010026784],"about_ca_topic_score_codex":0.004436755,"about_ca_topic_score_gemma":0.0075298883,"teacher_disagreement_score":0.00969342,"about_ca_system_score_codex":0.0006037088,"about_ca_system_score_gemma":0.0003521434,"threshold_uncertainty_score":0.03242773},"labels":[],"label_agreement":null},{"id":"W2079823208","doi":"10.1088/0004-637x/779/1/25","title":"GRAVITATIONAL LENS MODELS BASED ON SUBMILLIMETER ARRAY IMAGING OF<i>HERSCHEL</i>-SELECTED STRONGLY LENSED SUB-MILLIMETER GALAXIES AT<i>z</i>&gt; 1.5","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":223,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Smithsonian Astrophysical Observatory; Centre National de la Recherche Scientifique; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; Aspen Center for Physics; Centre National d’Etudes Spatiales; Academia Sinica; Ministerio de Ciencia, Tecnología e Innovación Productiva; UK Space Agency; Smithsonian Institution; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Millimeter; Astronomy; Gravitational lens; Submillimeter Array; Redshift; Lens (geology); South Pole Telescope; Quasar; Sky; Star formation; Optics","score_opus":0.009347369473195236,"score_gpt":0.19762731743663936,"score_spread":0.18827994796344413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079823208","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8656724,0.00093502324,0.11166135,0.00080782344,0.00004287739,0.000116853225,0.004769407,0.0012335881,0.014760718],"genre_scores_gemma":[0.98628795,0.00024049045,0.0081698075,0.000059872684,0.00002459742,0.000040071613,0.0018245047,0.0000632305,0.0032895263],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998099,0.00004230999,0.000012522359,0.000067535504,0.00002608468,0.00004160881],"domain_scores_gemma":[0.9990578,0.00036244927,0.000332501,0.000060550963,0.000096467724,0.00009018498],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000741626,0.00078788283,0.000354521,0.0009853556,0.0003628826,0.0012808773,0.0012297783,0.00083132024,0.0028312695],"category_scores_gemma":[0.0021910719,0.0004318795,0.0009600871,0.00064110104,0.00033437356,0.0010584076,0.00042047258,0.00035992425,0.0010336131],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017148384,0.00003765779,0.029326543,0.000030015108,0.0001371596,0.0000816711,0.000070692855,0.949328,0.001135007,0.007861672,0.0014943621,0.010325726],"study_design_scores_gemma":[0.000013053036,0.000016130958,0.005139057,0.000005519145,0.00002350517,0.000020683425,0.00001692875,0.9924799,0.00021148077,0.0016563183,0.0004076389,0.000009779974],"about_ca_topic_score_codex":0.060474977,"about_ca_topic_score_gemma":0.042907503,"teacher_disagreement_score":0.060474977,"about_ca_system_score_codex":0.002120517,"about_ca_system_score_gemma":0.0007038296,"threshold_uncertainty_score":0.12024599},"labels":[],"label_agreement":null},{"id":"W2079900698","doi":"10.1088/0004-637x/696/1/l89","title":"PAIRING OF SUPERMASSIVE BLACK HOLES IN UNEQUAL-MASS GALAXY MERGERS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy merger; Supermassive black hole; Galaxy; Redshift; Astronomy; Mass ratio","score_opus":0.008361970312595932,"score_gpt":0.2173545322001091,"score_spread":0.2089925618875132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079900698","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99846125,0.000038975577,0.00088131573,0.000037078917,0.000003695326,0.0000069044563,0.000018848472,0.000010635766,0.0005413481],"genre_scores_gemma":[0.9991654,0.000021987024,0.00064610544,0.000012894441,0.0000035261726,0.000004933062,0.000030767344,0.0000039758925,0.000110302884],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998093,0.0000641645,0.000008601267,0.000029302111,0.000023777233,0.00006487357],"domain_scores_gemma":[0.99865675,0.00049200153,0.00033586228,0.000094477895,0.0000627333,0.0003582259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00070642814,0.0003970575,0.0006190201,0.00052354287,0.0010621384,0.00091924967,0.00077271124,0.00074661395,0.0011502375],"category_scores_gemma":[0.0029798935,0.00042234804,0.000580961,0.000305117,0.0012438004,0.0011809624,0.001414139,0.0005940444,0.00011366819],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078892696,0.0003020561,0.099527255,0.00004959666,0.00017005861,0.0011681678,0.0006253214,0.8669956,0.009037164,0.016876431,0.0003672576,0.0040921755],"study_design_scores_gemma":[0.0002047973,0.00031916224,0.018028961,0.000010548542,0.000049115504,0.00017094573,0.00025731054,0.9718484,0.0024598937,0.006212374,0.0004094651,0.00002900328],"about_ca_topic_score_codex":0.008178915,"about_ca_topic_score_gemma":0.005186644,"teacher_disagreement_score":0.008178915,"about_ca_system_score_codex":0.000846052,"about_ca_system_score_gemma":0.00047723844,"threshold_uncertainty_score":0.01626265},"labels":[],"label_agreement":null},{"id":"W2079991755","doi":"10.1086/338112","title":"A<i>Far Ultraviolet Spectroscopic Explorer</i>Survey of Interstellar Molecular Hydrogen in the Small and Large Magellanic Clouds","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":219,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Milky Way; Large Magellanic Cloud; Astronomy; Stars; Small Magellanic Cloud; Far ultraviolet; Galaxy; Line-of-sight; Interstellar medium; Spectral line; Molecular cloud","score_opus":0.019340836385194494,"score_gpt":0.23121845928452128,"score_spread":0.2118776228993268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2079991755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97975516,0.00045353643,0.0012167258,0.00013609896,0.000008783132,0.00006528087,0.012202444,0.00022170396,0.005940288],"genre_scores_gemma":[0.9537346,0.0005216025,0.0077387434,0.00029459456,0.000060055834,0.00010575579,0.032804683,0.00004473509,0.0046951976],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988985,0.000013361328,0.0000044309136,0.000025416644,0.000033614953,0.00003336271],"domain_scores_gemma":[0.99956757,0.00002425257,0.00010742729,0.000037046655,0.000041685576,0.0002219666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028579682,0.00022258035,0.00011212232,0.0012922555,0.0003226902,0.00032351975,0.00025107976,0.00019034906,0.0014414205],"category_scores_gemma":[0.0001799959,0.00010513421,0.00015040641,0.00063092017,0.000090655834,0.00026122195,0.00042231963,0.00014284316,0.00043667434],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022405782,0.000231817,0.8858766,0.00006859789,0.00013029204,0.0002885257,0.00045793218,0.00035875395,0.050599873,0.00046463328,0.005701219,0.055597875],"study_design_scores_gemma":[0.000014314915,0.00009784139,0.98753905,0.000006985986,0.000017947443,0.00015551747,0.000092807495,0.00026673774,0.002040063,0.00006347878,0.009698864,0.0000063623897],"about_ca_topic_score_codex":0.0068438454,"about_ca_topic_score_gemma":0.01415994,"teacher_disagreement_score":0.0068438454,"about_ca_system_score_codex":0.00018844171,"about_ca_system_score_gemma":0.0002766913,"threshold_uncertainty_score":0.013607979},"labels":[],"label_agreement":null},{"id":"W2080029031","doi":"10.1086/318891","title":"Upper Limits on Periodic, Pulsed Radio Emission from the X-Ray Point Source in Cassiopeia A","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cassiopeia A; Pulsar; Supernova remnant; Point source; Luminosity; Neutron star; Flux (metallurgy); Crab Pulsar; Angular diameter","score_opus":0.015016710022387116,"score_gpt":0.23168910430801226,"score_spread":0.21667239428562515,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080029031","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94838893,0.009732014,0.008440496,0.0005003282,0.000037395686,0.00003717253,0.0013933626,0.00034573209,0.031124532],"genre_scores_gemma":[0.992619,0.0021345096,0.0027223446,0.00023281194,0.00009295117,0.00003693128,0.001442065,0.000029038023,0.000690338],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993042,0.00008008892,0.00007375886,0.00016036745,0.00024319066,0.00013853231],"domain_scores_gemma":[0.98925716,0.0072245803,0.0014217321,0.00070107525,0.000811646,0.0005837156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009608878,0.00045377424,0.0004918974,0.0022936282,0.00076237856,0.0015222781,0.00071027153,0.0011898618,0.0031438593],"category_scores_gemma":[0.006132396,0.00031966894,0.00032032392,0.0008473562,0.00077140424,0.0007077206,0.0016579737,0.00063324586,0.0009487329],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014894393,0.0002642122,0.700026,0.0013323049,0.0003521514,0.002821485,0.0018562174,0.0044695647,0.18943769,0.011152189,0.0047953534,0.08200332],"study_design_scores_gemma":[0.000056764096,0.00030569808,0.9407239,0.0003596448,0.00012529921,0.004138405,0.0003223369,0.0038162698,0.032849923,0.00651246,0.0107208295,0.00006856434],"about_ca_topic_score_codex":0.0023916126,"about_ca_topic_score_gemma":0.0023784041,"teacher_disagreement_score":0.0031438593,"about_ca_system_score_codex":0.0003989139,"about_ca_system_score_gemma":0.00018312197,"threshold_uncertainty_score":0.01051724},"labels":[],"label_agreement":null},{"id":"W2080054990","doi":"10.1088/0004-637x/745/2/171","title":"FAR-IR/SUBMILLIMETER SPECTROSCOPIC COSMOLOGICAL SURVEYS: PREDICTIONS OF INFRARED LINE LUMINOSITY FUNCTIONS FOR z &lt; 4 GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Active galactic nucleus; Galaxy; Luminous infrared galaxy; Luminosity function; Accretion (finance); Supermassive black hole; Luminosity; Star formation; Redshift; Infrared","score_opus":0.017702250857599664,"score_gpt":0.23388180632113076,"score_spread":0.2161795554635311,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080054990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926133,0.000035656794,0.005853855,0.00012980397,0.0000037270784,0.0000090242675,0.00032825297,0.00007652316,0.0009499601],"genre_scores_gemma":[0.99773514,0.000015996751,0.0016173183,0.00003269399,0.0000035965434,0.00000975563,0.0003119794,0.000015631762,0.00025784798],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99977165,0.0000887288,0.000006907626,0.000069653004,0.00002439823,0.000038574075],"domain_scores_gemma":[0.9982174,0.0008664779,0.00037475704,0.0001307298,0.00017450807,0.00023623485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018507333,0.0004083515,0.00025579197,0.0005743705,0.00033399698,0.0007908168,0.0009535608,0.0007718002,0.0012765798],"category_scores_gemma":[0.0042823297,0.0003164942,0.00074129784,0.00041576655,0.00038361308,0.0006632333,0.0003626402,0.00033948378,0.0003171802],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011729506,0.000070696864,0.3773878,0.00001288075,0.000059875605,0.00006098253,0.00006114512,0.6145802,0.0012239257,0.002465344,0.00040502063,0.003554736],"study_design_scores_gemma":[0.000022797016,0.000026774826,0.065908,0.0000070847173,0.000015921973,0.000021476826,0.000050191982,0.93240404,0.00036573576,0.0009969401,0.00017068049,0.000010320656],"about_ca_topic_score_codex":0.01896687,"about_ca_topic_score_gemma":0.009684973,"teacher_disagreement_score":0.01896687,"about_ca_system_score_codex":0.0011197482,"about_ca_system_score_gemma":0.00029306114,"threshold_uncertainty_score":0.03771299},"labels":[],"label_agreement":null},{"id":"W2080063950","doi":"10.1086/379760","title":"Physical Properties and Kinetic Structure of a Starless Core in Taurus Molecular Cloud","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Kinetic energy; Velocity gradient; Astronomy; Inner core; Mean kinetic temperature; Rotation (mathematics); Stars; Astrochemistry; Interstellar medium; Geometry; Galaxy","score_opus":0.011569931021033888,"score_gpt":0.22379026047903167,"score_spread":0.2122203294579978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080063950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987972,0.00009642066,0.000086156964,0.00004266092,0.000011863513,0.0000033406234,0.00007914415,0.000011016506,0.0008721508],"genre_scores_gemma":[0.9994118,0.000024341722,0.00004021267,0.000011337217,0.000017092634,0.0000010113417,0.000118150034,0.00000434195,0.0003717972],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999443,0.0000054236475,0.0000027178523,0.000015783738,0.000017071385,0.000014629694],"domain_scores_gemma":[0.9992404,0.00015557851,0.00013413254,0.000027625489,0.0002205831,0.00022172411],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010538927,0.00014130824,0.000267871,0.00050545414,0.00047096531,0.0005595397,0.00037887765,0.0003274644,0.002276868],"category_scores_gemma":[0.00092153635,0.000122049765,0.0001267768,0.00025134467,0.00027592812,0.0003629563,0.00026590354,0.0001737256,0.00033431844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023071663,0.0004230196,0.68766576,0.00021062062,0.00012713531,0.003910716,0.00044890423,0.011268195,0.26967567,0.002760466,0.0049244147,0.01627788],"study_design_scores_gemma":[0.00009859337,0.00027067825,0.95440596,0.000008267941,0.000042427175,0.00069734413,0.0002557832,0.030305704,0.0121133225,0.0008204624,0.0009561646,0.000025248799],"about_ca_topic_score_codex":0.0028388533,"about_ca_topic_score_gemma":0.0014989775,"teacher_disagreement_score":0.0028388533,"about_ca_system_score_codex":0.0002734483,"about_ca_system_score_gemma":0.00018260743,"threshold_uncertainty_score":0.0076168776},"labels":[],"label_agreement":null},{"id":"W2080073202","doi":"10.1088/0004-637x/717/1/121","title":"STAR FORMATION AND FEEDBACK IN SMOOTHED PARTICLE HYDRODYNAMIC SIMULATIONS. II. RESOLUTION EFFECTS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Dark matter; Star formation; Gravitational potential; Stellar mass; Halo; Dark matter halo; Smoothed-particle hydrodynamics; Stars","score_opus":0.0043201455612098495,"score_gpt":0.20475580320753772,"score_spread":0.20043565764632787,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080073202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878227,0.0001253557,0.007966522,0.00023649941,0.000035784684,0.00006574671,0.0004352992,0.0003363448,0.0029758126],"genre_scores_gemma":[0.9923834,0.000070407565,0.006198558,0.00009324329,0.00001621123,0.000058272693,0.00047952996,0.00010934157,0.00059098925],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99970067,0.00009836235,0.000019583144,0.00004062422,0.0000690384,0.00007186111],"domain_scores_gemma":[0.99705064,0.0017223585,0.00037638482,0.00020348055,0.00033640343,0.0003106758],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010550579,0.00067872583,0.00067031954,0.0006728916,0.0007174853,0.0007763274,0.0011789937,0.0011631637,0.0012875795],"category_scores_gemma":[0.0058893487,0.00045717557,0.00084266363,0.00045079683,0.0009559222,0.00088340614,0.00072794565,0.0008343351,0.00018779258],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015307195,0.00013739875,0.017098794,0.000046068704,0.00007304461,0.00013652231,0.00012295994,0.9753314,0.0023070297,0.0019837858,0.0004039075,0.0022060035],"study_design_scores_gemma":[0.000045129145,0.000037792423,0.0015287268,0.0000045799866,0.000008097108,0.000010461781,0.00001917588,0.9971975,0.0005394107,0.00045205132,0.00015000501,0.0000071244694],"about_ca_topic_score_codex":0.026163157,"about_ca_topic_score_gemma":0.016006894,"teacher_disagreement_score":0.026163157,"about_ca_system_score_codex":0.0013530196,"about_ca_system_score_gemma":0.0011709855,"threshold_uncertainty_score":0.052021742},"labels":[],"label_agreement":null},{"id":"W2080077537","doi":"10.1086/308424","title":"V633 Cassiopeiae (LkHα 198) and V628 Cassiopeiae (MWC 1080) Revisited!","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; Astrophysics; Millimeter; Spectral energy distribution; Stars; Young stellar object; James Clerk Maxwell Telescope; Emissivity; T Tauri star; Spectral index; Astronomy; Position angle; Molecular cloud; Star formation; Spectral line; Optics; Galaxy","score_opus":0.008940099775429733,"score_gpt":0.23613120704822232,"score_spread":0.2271911072727926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080077537","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9891222,0.0009675151,0.00021587398,0.0002761779,0.000029531402,0.000011078967,0.00050871976,0.000048583857,0.0088203885],"genre_scores_gemma":[0.9964504,0.00024758055,0.00040058492,0.00010748549,0.000027433916,0.000005531974,0.0008047636,0.000015690832,0.0019404866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998871,0.0000048817274,0.0000037816033,0.000041689,0.000019220543,0.00004325786],"domain_scores_gemma":[0.99982446,0.0000076284,0.00007620493,0.000017133645,0.00002667748,0.00004792202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011750311,0.00027307495,0.0002147028,0.00055616786,0.0009719659,0.0006468235,0.00023111433,0.00038328668,0.0036186546],"category_scores_gemma":[0.00015882631,0.00010678741,0.00018083057,0.0008547356,0.00032249585,0.0003022193,0.00044453266,0.0004092133,0.0010905478],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033559816,0.000048162867,0.9179699,0.000082598875,0.00008552494,0.0027041023,0.0008938562,0.00021663259,0.033210002,0.0015459474,0.004845644,0.038062017],"study_design_scores_gemma":[0.000008981629,0.00002362718,0.9857927,0.000015869651,0.000016999935,0.0016820285,0.0003380902,0.00016815256,0.0008541764,0.0002846018,0.010809088,0.0000056346053],"about_ca_topic_score_codex":0.024564499,"about_ca_topic_score_gemma":0.0357972,"teacher_disagreement_score":0.024564499,"about_ca_system_score_codex":0.00045111816,"about_ca_system_score_gemma":0.00026282278,"threshold_uncertainty_score":0.048843026},"labels":[],"label_agreement":null},{"id":"W2080161165","doi":"10.1086/427256","title":"The DEEP Groth Strip Galaxy Redshift Survey. III. Redshift Catalog and Properties of Galaxies","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":169,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Redshift; Galaxy; Bulge; Lenticular galaxy; Elliptical galaxy; Redshift survey; Red shift; Brightest cluster galaxy; Galaxy formation and evolution","score_opus":0.011618528039804711,"score_gpt":0.20840289323830657,"score_spread":0.19678436519850187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080161165","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.060139526,0.00056545285,0.0024024814,0.00031932048,0.00006804508,0.00074629707,0.90483946,0.0014649997,0.02945452],"genre_scores_gemma":[0.051366977,0.000349017,0.0058535486,0.000248378,0.0000789804,0.00060901995,0.92965347,0.00022689321,0.011613731],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9992544,0.000084904575,0.000053836775,0.00017182154,0.00030660108,0.00012833235],"domain_scores_gemma":[0.9980116,0.00009262643,0.00051330146,0.0004574865,0.00053687044,0.00038804606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009278123,0.0007496625,0.0005280537,0.004653188,0.00042559134,0.00089620677,0.00090659334,0.0003700395,0.014178029],"category_scores_gemma":[0.001339209,0.0003458302,0.0003302752,0.0047914,0.00021456773,0.0006608501,0.001619541,0.0007238153,0.012488494],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050134317,0.00019761753,0.3345328,0.0007107159,0.00029775128,0.00022223103,0.0006789004,0.0008516479,0.010002958,0.0038343736,0.5541138,0.09405584],"study_design_scores_gemma":[0.00010921419,0.000078425015,0.7369486,0.00009468455,0.000038488022,0.0001904566,0.00018528932,0.00045496027,0.0010788249,0.00062362646,0.26017323,0.000024216077],"about_ca_topic_score_codex":0.019812198,"about_ca_topic_score_gemma":0.019615218,"teacher_disagreement_score":0.019812198,"about_ca_system_score_codex":0.0006437951,"about_ca_system_score_gemma":0.0009262551,"threshold_uncertainty_score":0.047430277},"labels":[],"label_agreement":null},{"id":"W2080163811","doi":"10.1088/0004-637x/768/1/55","title":"<i>HERSCHEL</i>/SPIRE SUBMILLIMETER SPECTRA OF LOCAL ACTIVE GALAXIES<sup>,</sup>","year":2013,"lang":"fr","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Centre National de la Recherche Scientifique; Imperial College London; Agenzia Spaziale Italiana; Università degli Studi di Padova; Jet Propulsion Laboratory; Centre National d’Etudes Spatiales; Cardiff University; University of Sussex; National Aeronautics and Space Administration; California Institute of Technology; University of Lethbridge; UK Space Agency","keywords":"Physics; Galaxy; Astrophysics; Spire (mollusc); Spectral line; Emission spectrum; Radiative transfer; Line (geometry); Luminous infrared galaxy; Star formation; Millimeter; Astronomy","score_opus":0.008965778081573198,"score_gpt":0.21722654418267084,"score_spread":0.20826076610109764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080163811","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.35244718,0.0033892943,0.008782545,0.004687237,0.0018739214,0.00011163789,0.53617406,0.010454407,0.082079716],"genre_scores_gemma":[0.61739737,0.0012972526,0.0127454465,0.002254673,0.0010786813,0.0001118396,0.32814896,0.003283115,0.0336827],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9998834,0.0000069605626,0.000007175949,0.000026495027,0.00004373585,0.00003219557],"domain_scores_gemma":[0.9993767,0.00009200166,0.00014537708,0.00009404717,0.00014916307,0.00014281317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003822835,0.00046397615,0.00029546543,0.003543369,0.00044486797,0.00058660214,0.00055617315,0.00064073276,0.04098081],"category_scores_gemma":[0.00058114424,0.00026692642,0.0006229405,0.0022367097,0.0001759436,0.0006012036,0.0005825376,0.00053911237,0.009544782],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015827123,0.00016607852,0.13711923,0.0009103811,0.00050459465,0.000615492,0.00043740528,0.0027270585,0.15670687,0.0024705622,0.6100233,0.08673629],"study_design_scores_gemma":[0.000052101874,0.000057216825,0.90891486,0.00005536334,0.00012737072,0.00035821376,0.00023927308,0.0017504933,0.014028916,0.0010699424,0.07329499,0.00005128291],"about_ca_topic_score_codex":0.006445518,"about_ca_topic_score_gemma":0.015761776,"teacher_disagreement_score":0.04098081,"about_ca_system_score_codex":0.00036480563,"about_ca_system_score_gemma":0.00023118287,"threshold_uncertainty_score":0.1370945},"labels":[],"label_agreement":null},{"id":"W2080253828","doi":"10.1086/312802","title":"Photospheric Metals in the [ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Spectrum of the Subdwarf B Star PG 0749+658","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Subdwarf; Astrophysics; Stellar atmosphere; Spectral line; Ultraviolet; Radiative transfer; Star (game theory); Astronomy; Stars; Optics","score_opus":0.009657592494438315,"score_gpt":0.21559305630501704,"score_spread":0.20593546381057873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080253828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972249,0.000048840975,0.00009220051,0.000021919494,0.0000021628275,0.0000014766458,0.000715312,0.000028069382,0.0018650788],"genre_scores_gemma":[0.99749243,0.000042605472,0.00026212362,0.000021762282,0.0000046737005,0.000003276967,0.001833601,0.000008585305,0.00033107417],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999821,0.000001395206,8.126981e-7,0.000005740132,0.0000047181074,0.0000051777565],"domain_scores_gemma":[0.99994004,0.0000073502733,0.000019135432,0.000006920652,0.000008947273,0.000017545615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000041335596,0.00016371647,0.00009739688,0.00051692844,0.00019789585,0.00020957974,0.00012667445,0.00015918292,0.0020743664],"category_scores_gemma":[0.00009924931,0.00006735366,0.00008340786,0.00031283734,0.00007991887,0.00009067528,0.00017640537,0.00010304953,0.00055515737],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004688995,0.000093363706,0.88054323,0.00004677635,0.00008414517,0.00049898913,0.00019934484,0.0019427841,0.09427642,0.0005867466,0.0040162895,0.01724294],"study_design_scores_gemma":[0.000013362792,0.000027659476,0.9961578,0.000004120961,0.000009980951,0.00011512731,0.000039963,0.0007598124,0.0013330355,0.00013331625,0.0014036135,0.0000021339827],"about_ca_topic_score_codex":0.0020795185,"about_ca_topic_score_gemma":0.0033307786,"teacher_disagreement_score":0.0020795185,"about_ca_system_score_codex":0.00012288989,"about_ca_system_score_gemma":0.000031557476,"threshold_uncertainty_score":0.006939411},"labels":[],"label_agreement":null},{"id":"W2080350480","doi":"10.1088/0004-637x/763/1/55","title":"CHANGES OF DUST OPACITY WITH DENSITY IN THE ORION A MOLECULAR CLOUD","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":139,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Opacity; Molecular cloud; Cloud computing; Astrophysics; Astronomy; Physics; Environmental science; Stars; Computer science; Optics; Operating system","score_opus":0.008993142845543754,"score_gpt":0.21347853204761436,"score_spread":0.2044853892020706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080350480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963427,0.00005197877,0.000105728905,0.0000072704433,4.106486e-7,0.0000012987091,0.000050217513,0.000008955036,0.0001398454],"genre_scores_gemma":[0.99956197,0.000030958246,0.00018355707,0.0000039461975,0.000001682576,0.0000024596284,0.00010286872,0.0000038962075,0.0001087158],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999008,0.000008883191,0.000006136213,0.000040067738,0.000020979272,0.000023220322],"domain_scores_gemma":[0.9994518,0.00012992512,0.00020028006,0.000048618695,0.000111111985,0.000058228263],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016969367,0.00022242124,0.0001866743,0.0005790129,0.0002906739,0.00043660172,0.0003314982,0.0002253321,0.00053498015],"category_scores_gemma":[0.00075987325,0.00024049355,0.0001736885,0.0003622496,0.00024791362,0.00038879339,0.00035965932,0.00026237287,0.00011246626],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021740214,0.00009352213,0.81008494,0.00002773921,0.00005068303,0.00028821765,0.0003621203,0.0029276789,0.18005504,0.00017389467,0.00006506657,0.0056535588],"study_design_scores_gemma":[0.0000046646715,0.00004256276,0.9910458,0.0000031332297,0.000008836918,0.000078862104,0.00007398566,0.0029415186,0.00556849,0.000053827207,0.00017255977,0.0000057476987],"about_ca_topic_score_codex":0.008457183,"about_ca_topic_score_gemma":0.007058767,"teacher_disagreement_score":0.008457183,"about_ca_system_score_codex":0.00046553338,"about_ca_system_score_gemma":0.00009407087,"threshold_uncertainty_score":0.0168159},"labels":[],"label_agreement":null},{"id":"W2080362858","doi":"10.1088/0004-637x/759/2/98","title":"BREAKS IN THIN AND THICK DISKS OF EDGE-ON GALAXIES IMAGED IN THE<i>SPITZER</i>SURVEY OF STELLAR STRUCTURE IN GALAXIES (S<sup>4</sup>G)","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Princeton University","keywords":"Physics; Astrophysics; Thin disk; Thick disk; Galaxy; Luminosity; RADIUS; Disc; Stellar mass; Astronomy; Galaxy formation and evolution; Star formation; Halo","score_opus":0.010126749528855545,"score_gpt":0.22545212556361974,"score_spread":0.2153253760347642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080362858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988011,0.00014032524,0.00039396004,0.0000061694836,0.0000011120146,0.000003523667,0.00038909097,0.000019677724,0.0002450174],"genre_scores_gemma":[0.9975611,0.00006082686,0.00084990455,0.0000073005976,0.000003724718,0.0000030981028,0.001350012,0.000015773925,0.00014827681],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997316,0.000027583033,0.00002616111,0.00008202801,0.00005411539,0.0000784093],"domain_scores_gemma":[0.99876815,0.0001901883,0.0005185433,0.00014309064,0.0001735778,0.00020645926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039455816,0.0002959814,0.00021919927,0.0020039035,0.0002478295,0.0006577775,0.00029071604,0.00038925878,0.0008924111],"category_scores_gemma":[0.0010754603,0.00030149118,0.000370013,0.000867842,0.00035369207,0.0004875403,0.00059412676,0.00024303512,0.00040731172],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013692773,0.00001563423,0.9738807,0.000021841803,0.00006173311,0.00012533969,0.00028374544,0.00051961554,0.01790239,0.000064106265,0.00011734991,0.0068706106],"study_design_scores_gemma":[0.0000010698692,0.000013706514,0.99781775,0.0000033810081,0.000013736259,0.00012125692,0.00008686725,0.0007098356,0.0010713398,0.000029075942,0.00012948751,0.0000025006377],"about_ca_topic_score_codex":0.0042807343,"about_ca_topic_score_gemma":0.008998286,"teacher_disagreement_score":0.0042807343,"about_ca_system_score_codex":0.00033232788,"about_ca_system_score_gemma":0.000082776045,"threshold_uncertainty_score":0.0085116625},"labels":[],"label_agreement":null},{"id":"W2080397780","doi":"10.1086/337988","title":"Metastudy of the Spiral Structure of Our Home Galaxy","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Milky Way; Spiral galaxy; Astrophysics; Logarithmic spiral; Galaxy; Sagittarius; Spiral (railway); RADIUS; Grand design spiral galaxy; Astronomy; Irregular galaxy; Barred spiral galaxy; Interacting galaxy; Dwarf galaxy; Geometry","score_opus":0.013070093922766193,"score_gpt":0.2177263428586686,"score_spread":0.2046562489359024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080397780","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9749204,0.00092736684,0.0056280564,0.00039647977,0.000013230322,0.0000047742897,0.0007910489,0.00017909173,0.017139502],"genre_scores_gemma":[0.99729854,0.0002765609,0.00094259507,0.00003635149,0.000010056317,0.000002487606,0.0003696055,0.000021247946,0.0010425604],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999187,0.000014428661,0.0000028526483,0.00003794539,0.000014896773,0.00001119097],"domain_scores_gemma":[0.99981004,0.00004216643,0.00005396461,0.000055422443,0.000023091243,0.00001522165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013691097,0.00015374906,0.00019686398,0.00094167347,0.00031775195,0.0012035392,0.00026203814,0.00021023901,0.004033673],"category_scores_gemma":[0.000820543,0.000126504,0.00041851035,0.0009822184,0.00046546475,0.0007478266,0.00037718978,0.0003342786,0.00034459602],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033962246,0.000034318437,0.8021286,0.0001895639,0.00055315334,0.00058374484,0.0038776938,0.010395392,0.025186485,0.045558307,0.0032279217,0.107925214],"study_design_scores_gemma":[0.000014294726,0.000082432605,0.9485223,0.000052725183,0.00020179733,0.00065992994,0.0021496634,0.015147797,0.0031332474,0.016547948,0.013450192,0.000037633832],"about_ca_topic_score_codex":0.011954,"about_ca_topic_score_gemma":0.01998844,"teacher_disagreement_score":0.011954,"about_ca_system_score_codex":0.0009410402,"about_ca_system_score_gemma":0.00019752298,"threshold_uncertainty_score":0.023768842},"labels":[],"label_agreement":null},{"id":"W2080579076","doi":"10.1088/0004-637x/765/2/151","title":"MULTIBAND STUDIES OF THE OPTICAL PERIODIC MODULATION IN THE X-RAY BINARY SAX J1808.4–3658 DURING ITS QUIESCENCE AND 2008 OUTBURST","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Millisecond pulsar; Light curve; Neutron star; Amplitude; Accretion (finance); Modulation (music); Pulsar; Binary number; X-ray binary; Astronomy; Optics","score_opus":0.020565517125317602,"score_gpt":0.24769315528390964,"score_spread":0.22712763815859205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080579076","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993667,0.000047410707,0.0002134478,0.000007768491,0.000001196369,0.0000023827336,0.0000393897,0.0000064490205,0.00031529358],"genre_scores_gemma":[0.9993968,0.000034450848,0.00032101604,0.0000051551715,0.0000033624324,0.0000027390686,0.00009108909,0.0000032784424,0.00014207269],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996233,0.0000036047882,0.0000022325612,0.000011367264,0.000010465406,0.000009993553],"domain_scores_gemma":[0.999811,0.000034032946,0.000090992406,0.000009905228,0.000021297841,0.00003280353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001100859,0.00011974099,0.00013748778,0.0004269437,0.00023132421,0.00021995905,0.00013598653,0.00016021718,0.00045735863],"category_scores_gemma":[0.00027802275,0.0001300581,0.00012137269,0.0002542691,0.00015447882,0.00018752724,0.00021811933,0.00019861171,0.000093338516],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006700318,0.00021708416,0.66275555,0.00009303397,0.00009584576,0.0011928227,0.00085634354,0.003853717,0.306321,0.0005445559,0.00031185977,0.02308813],"study_design_scores_gemma":[0.000009228284,0.0001407793,0.98879236,0.000005883878,0.000020260535,0.0003802305,0.00015784407,0.0043496527,0.005456217,0.00011074728,0.00056940253,0.0000073973642],"about_ca_topic_score_codex":0.0014850053,"about_ca_topic_score_gemma":0.003941719,"teacher_disagreement_score":0.0014850053,"about_ca_system_score_codex":0.00018158146,"about_ca_system_score_gemma":0.000073285235,"threshold_uncertainty_score":0.002952695},"labels":[],"label_agreement":null},{"id":"W2080610645","doi":"10.1088/0004-637x/696/2/1871","title":"GRB 080503: IMPLICATIONS OF A NAKED SHORT GAMMA-RAY BURST DOMINATED BY EXTENDED EMISSION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":210,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; U.S. Department of Energy; National Science Foundation","keywords":"Afterglow; Gamma-ray burst; Physics; Astrophysics; Brightness; Astronomy; Supernova; Luminosity; Galaxy","score_opus":0.00902935842544787,"score_gpt":0.25045884866536733,"score_spread":0.24142949023991947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080610645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9489396,0.0029050855,0.0032283564,0.009300561,0.0009005193,0.0000326127,0.0011966195,0.00031992426,0.033176683],"genre_scores_gemma":[0.99606246,0.0005418811,0.0005233085,0.0006174628,0.00034297406,0.0000061040187,0.000336602,0.00002920299,0.0015400201],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998258,0.00002599517,0.00003450115,0.000042002535,0.000028161545,0.00004363318],"domain_scores_gemma":[0.99835193,0.0003327252,0.00047598116,0.00023247197,0.00020574967,0.00040118422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007697645,0.0005519226,0.0005336076,0.0008268129,0.0009434485,0.0029164099,0.0010699461,0.0028670004,0.007988494],"category_scores_gemma":[0.0024630385,0.00022678029,0.00045621433,0.0010926734,0.0018380204,0.0016423403,0.0013282229,0.0014492391,0.0017807658],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.008535122,0.00092775235,0.64124566,0.0006639648,0.00027201418,0.08074526,0.0009717148,0.0070357365,0.08606681,0.061825518,0.033077158,0.07863326],"study_design_scores_gemma":[0.00089187926,0.00047763682,0.7565649,0.00027664358,0.00026911986,0.08550404,0.0020753324,0.016624901,0.005938073,0.11557971,0.015510746,0.00028702093],"about_ca_topic_score_codex":0.0047322907,"about_ca_topic_score_gemma":0.0024221116,"teacher_disagreement_score":0.007988494,"about_ca_system_score_codex":0.00081909925,"about_ca_system_score_gemma":0.0005647498,"threshold_uncertainty_score":0.02672416},"labels":[],"label_agreement":null},{"id":"W2080630737","doi":"10.1086/498242","title":"A Pre‐Protostellar Core in L1551. II. State of Dynamical and Chemical Evolution","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Radiative transfer; Star formation; Protostar; Gravitational collapse; Molecular cloud; Accretion (finance); Line (geometry); Astronomy; Stars; Geometry; Optics","score_opus":0.005140508299221825,"score_gpt":0.2176594748302345,"score_spread":0.21251896653101268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080630737","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988991,0.00015417078,0.00007025035,0.000012772304,0.0000011447092,0.0000034610703,0.00014401905,0.0000060817924,0.00070895057],"genre_scores_gemma":[0.9994566,0.000030997842,0.00007548265,0.000008902409,0.0000012839712,0.0000016939744,0.00019708496,0.0000016975353,0.00022625897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999969,0.000002653253,0.0000019732652,0.000008716906,0.0000054153415,0.000012220081],"domain_scores_gemma":[0.99987495,0.000012676752,0.000048464626,0.000007466335,0.000017954777,0.00003833568],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009527335,0.00013794871,0.00013030626,0.00026423912,0.0002664334,0.00039930842,0.00030085692,0.00015852098,0.00063644384],"category_scores_gemma":[0.000254369,0.000093011826,0.0001049407,0.00013434172,0.00021957955,0.00019888462,0.0002451116,0.00016071921,0.0002372375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009653493,0.0001429729,0.7733818,0.00011971585,0.00008435064,0.0013650673,0.0005338303,0.0077307643,0.19403583,0.0021320055,0.0008497679,0.018658534],"study_design_scores_gemma":[0.000009735901,0.0000763574,0.9872162,0.000011800355,0.000015358306,0.00021971927,0.00012978539,0.005065041,0.00623386,0.00017667368,0.00083716563,0.0000082566075],"about_ca_topic_score_codex":0.022238243,"about_ca_topic_score_gemma":0.018450923,"teacher_disagreement_score":0.022238243,"about_ca_system_score_codex":0.0013085409,"about_ca_system_score_gemma":0.00016029282,"threshold_uncertainty_score":0.044217646},"labels":[],"label_agreement":null},{"id":"W2080641454","doi":"10.1086/380483","title":"On the Structure of Quasi‐universal Jets for Gamma‐Ray Bursts","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Gamma-ray burst; Physics; Afterglow; Jet (fluid); Viewing angle; Astrophysics; Gaussian; Power law; Light curve; Isotropy; Function (biology); Statistical physics; Optics; Mechanics; Statistics","score_opus":0.009449286228404,"score_gpt":0.22504696058563217,"score_spread":0.21559767435722818,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080641454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9628407,0.0013066219,0.029872585,0.0004886738,0.000026608632,0.000024261353,0.00015616138,0.00029713148,0.00498728],"genre_scores_gemma":[0.994776,0.00050420646,0.004167436,0.00005726868,0.000060506936,0.000013924268,0.00012922939,0.000052639218,0.00023884467],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99970573,0.000082698876,0.000017836512,0.000073559095,0.000041223582,0.00007887601],"domain_scores_gemma":[0.9915869,0.003814324,0.002398025,0.0010789918,0.0004355291,0.0006863122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012903179,0.00045163318,0.0006123658,0.0016420903,0.00078651425,0.0032478261,0.0010347678,0.00087688275,0.0017729257],"category_scores_gemma":[0.008426939,0.00047895923,0.00079079944,0.0010414583,0.0026317653,0.0027742893,0.0011072567,0.00070987537,0.00021723559],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077876926,0.00034082978,0.26259822,0.00028692425,0.0001627851,0.002296203,0.0026706103,0.16139601,0.01943845,0.49116954,0.0023226505,0.05653899],"study_design_scores_gemma":[0.00011721131,0.00019333836,0.13220444,0.00010004517,0.000091403774,0.001260166,0.00046415083,0.5145,0.0016914821,0.34735334,0.001913715,0.00011069513],"about_ca_topic_score_codex":0.0015769153,"about_ca_topic_score_gemma":0.0011128755,"teacher_disagreement_score":0.0032478261,"about_ca_system_score_codex":0.0010366718,"about_ca_system_score_gemma":0.00053111714,"threshold_uncertainty_score":0.0075216293},"labels":[],"label_agreement":null},{"id":"W2080738600","doi":"10.1088/0004-637x/748/2/102","title":"GEMINI SPECTROSCOPIC SURVEY OF YOUNG STAR CLUSTERS IN MERGING/INTERACTING GALAXIES. IV. STEPHAN's QUINTET","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Star cluster; Cluster (spacecraft); Galaxy cluster; Galaxy; Galaxy groups and clusters; Population; Star formation; Dwarf galaxy","score_opus":0.012573392535692895,"score_gpt":0.24665207037102463,"score_spread":0.23407867783533173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080738600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99604475,0.00018314857,0.00010351191,0.00005806353,0.0000025947259,0.000017153157,0.0010102534,0.000026353595,0.0025541633],"genre_scores_gemma":[0.9956708,0.00009812761,0.00038000013,0.000032234184,0.0000052678206,0.000008927759,0.0018141263,0.000009145954,0.001981374],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987364,0.000009535178,0.000004366014,0.00003769561,0.000041318795,0.0000333353],"domain_scores_gemma":[0.9996538,0.000017881692,0.000092514056,0.000029612529,0.00006503313,0.00014111499],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001547011,0.0001882955,0.00015412379,0.001295557,0.0006606734,0.00030343476,0.00045904852,0.00011007383,0.0025763786],"category_scores_gemma":[0.00029060242,0.00011850151,0.000108496,0.0010540024,0.00017337594,0.00025154845,0.00077545864,0.00016404338,0.00040718596],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006451498,0.00004732335,0.9723337,0.00003302398,0.000023909619,0.0005256706,0.0017211143,0.00009024222,0.008068704,0.00034957952,0.0018793257,0.014862856],"study_design_scores_gemma":[0.0000020594498,0.00002319094,0.9958139,0.0000036679785,0.000004224677,0.00028638696,0.0003226498,0.00014902744,0.0003054627,0.000035797977,0.0030509802,0.0000026316661],"about_ca_topic_score_codex":0.032126814,"about_ca_topic_score_gemma":0.08564919,"teacher_disagreement_score":0.032126814,"about_ca_system_score_codex":0.0003603553,"about_ca_system_score_gemma":0.0002826101,"threshold_uncertainty_score":0.06387961},"labels":[],"label_agreement":null},{"id":"W2080774701","doi":"10.1086/309504","title":"High‐Resolution Imaging of Molecular Gas and Dust in the Antennae (NGC 4038/39): Super Giant Molecular Complexes","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":155,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Stars; Star formation; Globular cluster; Star cluster; Galaxy; Astronomy; Molecular cloud; Infrared; Hubble space telescope","score_opus":0.004646923705253558,"score_gpt":0.19721714400441673,"score_spread":0.19257022029916318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2080774701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747604,0.000058714348,0.00009811005,0.000033830383,0.0000015029293,0.0000044383846,0.0002545604,0.000024597695,0.002048233],"genre_scores_gemma":[0.9978125,0.00006415983,0.00080986647,0.000025232928,0.00000758078,0.000008578663,0.00039961544,0.000010349362,0.00086204737],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994147,0.0000027057722,0.0000016654874,0.00001740885,0.000016210684,0.00002047939],"domain_scores_gemma":[0.99990463,0.000007091868,0.000023144554,0.000009186439,0.000010708759,0.000045176374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007356026,0.00016941334,0.00011002105,0.00068703777,0.00023416641,0.00024842282,0.00024774254,0.0002195626,0.0016789488],"category_scores_gemma":[0.00011932405,0.00015939753,0.00008838978,0.00033493698,0.00012727438,0.00014957317,0.00035086766,0.00017156058,0.00030635757],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022260593,0.000077225464,0.12212,0.00006790522,0.00004705313,0.0013644074,0.0006813106,0.00092125114,0.85793614,0.00038645449,0.0015237983,0.014651772],"study_design_scores_gemma":[0.000020927186,0.00005271676,0.98652875,0.00001087875,0.000011715355,0.000977872,0.00019291138,0.0013335058,0.007472999,0.00015343157,0.003236213,0.000008025542],"about_ca_topic_score_codex":0.0054883556,"about_ca_topic_score_gemma":0.010841139,"teacher_disagreement_score":0.0054883556,"about_ca_system_score_codex":0.0003139458,"about_ca_system_score_gemma":0.0000886545,"threshold_uncertainty_score":0.010912836},"labels":[],"label_agreement":null},{"id":"W2081054777","doi":"10.1086/522337","title":"Further Evidence That the Redshifts of AGN Galaxies May Contain Intrinsic Components","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Redshift; Luminosity; Galaxy; Radio galaxy; Star formation; Active galactic nucleus; Luminosity function","score_opus":0.021361243572314233,"score_gpt":0.2444403051901012,"score_spread":0.22307906161778698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081054777","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8197982,0.0023873097,0.113793224,0.0044861804,0.00017752207,0.00006590133,0.0011003488,0.0012953269,0.056895982],"genre_scores_gemma":[0.98674273,0.0004982631,0.006212995,0.00050263794,0.00007001204,0.000011056858,0.0006459719,0.000053644835,0.005262697],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99956185,0.000058554775,0.000023501441,0.00016798999,0.00012136789,0.00006672576],"domain_scores_gemma":[0.99615496,0.0014745995,0.0010433337,0.0007336357,0.00032499342,0.00026838193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010775273,0.0005753384,0.00036592875,0.0009270771,0.00043973056,0.001451641,0.0012116029,0.0007456647,0.00878813],"category_scores_gemma":[0.003608743,0.0003017149,0.0005811235,0.001100462,0.00096787256,0.002341581,0.0009866693,0.0010623949,0.0015162056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008034087,0.00023343707,0.6709602,0.0007011669,0.00028781377,0.0011227827,0.0019514676,0.008429163,0.046882205,0.17682947,0.0050642616,0.08673462],"study_design_scores_gemma":[0.00009638207,0.00080372306,0.79225886,0.0000687126,0.00022004583,0.006352187,0.0010480593,0.05099703,0.01213302,0.09253936,0.043388676,0.00009395232],"about_ca_topic_score_codex":0.0032952402,"about_ca_topic_score_gemma":0.0034155503,"teacher_disagreement_score":0.00878813,"about_ca_system_score_codex":0.00048119357,"about_ca_system_score_gemma":0.00022585415,"threshold_uncertainty_score":0.029399276},"labels":[],"label_agreement":null},{"id":"W2081061179","doi":"10.1086/424811","title":"The VSOP 5 GHz Active Galactic Nucleus Survey. IV. The Angular Size/Brightness Temperature Distribution","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Very-long-baseline interferometry; Physics; Brightness; Brightness temperature; Astrophysics; Active galactic nucleus; Angular diameter; Angular resolution (graph drawing); Radio telescope; Telescope; Astronomy; Satellite; Amplitude; Optics; Galaxy; Stars","score_opus":0.0052516114220547555,"score_gpt":0.21350504015068747,"score_spread":0.20825342872863273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081061179","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.11340696,0.0029928572,0.0040671118,0.0011620083,0.00026159402,0.00047620575,0.8221914,0.00094452366,0.054497305],"genre_scores_gemma":[0.2118777,0.001821688,0.007378569,0.0005731397,0.00020378185,0.00036083424,0.7429529,0.0002684326,0.03456298],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99976474,0.00003693771,0.00001486529,0.00004185028,0.00009356124,0.00004799595],"domain_scores_gemma":[0.99952817,0.000030296944,0.00009458703,0.00010002241,0.00013275899,0.00011414358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043572503,0.00034266352,0.00019110377,0.0022054738,0.0002815843,0.00050154293,0.00057665765,0.00024613287,0.0099373],"category_scores_gemma":[0.00072569627,0.00018527768,0.00017136536,0.0031881733,0.00014124774,0.0003978522,0.0009801754,0.00027444342,0.004624173],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005030321,0.00010735942,0.3023046,0.00046005024,0.00017049366,0.00020450079,0.00030341896,0.0010354014,0.004261114,0.0031453588,0.47995982,0.20754495],"study_design_scores_gemma":[0.00006954589,0.000052936794,0.5759205,0.000067225345,0.000043925585,0.00017779823,0.0001509904,0.00026021415,0.0010659605,0.0006924932,0.4214893,0.000009177479],"about_ca_topic_score_codex":0.03947475,"about_ca_topic_score_gemma":0.04472922,"teacher_disagreement_score":0.03947475,"about_ca_system_score_codex":0.00066638086,"about_ca_system_score_gemma":0.0006846364,"threshold_uncertainty_score":0.07848996},"labels":[],"label_agreement":null},{"id":"W2081182230","doi":"10.1086/341059","title":"Cosmological Aspects of Gamma‐Ray Bursts: Luminosity Evolution and an Estimate of the Star Formation Rate at High Redshifts","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":164,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Astrophysics; Physics; Redshift; Gamma-ray burst; Luminosity; Star formation; Luminosity function; Population; Astronomy; Stars; Galaxy","score_opus":0.013818994069289254,"score_gpt":0.22544169153031107,"score_spread":0.21162269746102183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081182230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951167,0.00023754149,0.003660885,0.000037468,0.0000012100343,0.000006405906,0.00016976842,0.00004635327,0.00072358997],"genre_scores_gemma":[0.9978617,0.000118319316,0.0015811071,0.000005911279,0.0000052806504,0.000003572617,0.0002920519,0.000014240431,0.00011789548],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981195,0.00006785443,0.00001411822,0.000046125464,0.000035764348,0.000024269071],"domain_scores_gemma":[0.9963186,0.0014722202,0.0015075275,0.00031660515,0.0001997857,0.0001852796],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014302433,0.00031890033,0.00026319968,0.0023633994,0.0003162608,0.0009395893,0.00045308637,0.00051873026,0.00068328384],"category_scores_gemma":[0.006336312,0.00032792863,0.0003885962,0.0017458725,0.00045282143,0.00079635537,0.0005423752,0.0004347569,0.00025700423],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009254801,0.000045133304,0.9627448,0.000038623522,0.000099002646,0.00010938046,0.00033607782,0.01127984,0.011136541,0.0029060645,0.00011129862,0.011100743],"study_design_scores_gemma":[0.000005507344,0.000020814114,0.97062206,0.000008275588,0.000030373905,0.00024852893,0.000054665576,0.02568515,0.00188371,0.0011437391,0.00028077062,0.000016432658],"about_ca_topic_score_codex":0.004214031,"about_ca_topic_score_gemma":0.003911406,"teacher_disagreement_score":0.004214031,"about_ca_system_score_codex":0.0005681785,"about_ca_system_score_gemma":0.00015533107,"threshold_uncertainty_score":0.008378983},"labels":[],"label_agreement":null},{"id":"W2081250528","doi":"10.1086/379108","title":"Testing the Binary Black Hole Paradigm through the Fe K Line Profile: Application to 3C 273","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Active galactic nucleus; Binary number; Precession; Line (geometry); Binary black hole; Galaxy; Black hole (networking); Signature (topology); Variation (astronomy); Enhanced Data Rates for GSM Evolution","score_opus":0.027155807110938252,"score_gpt":0.2620176218780025,"score_spread":0.23486181476706422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081250528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977176,0.000021467671,0.0007619952,0.00004238508,0.0000020578846,0.000011602274,0.00007526055,0.000021409931,0.0013463804],"genre_scores_gemma":[0.9988366,0.000020122388,0.0009491004,0.00001477347,0.0000029163325,0.0000051261045,0.000048047612,0.000010331048,0.00011314683],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999099,0.000012089525,0.0000031155512,0.00003114112,0.00002349826,0.00002034633],"domain_scores_gemma":[0.99963176,0.00008106087,0.00008894707,0.00006152358,0.00006310907,0.00007363388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002923972,0.00030313258,0.00027236098,0.0005227495,0.00081593374,0.000661531,0.0005751437,0.0006004013,0.0007538825],"category_scores_gemma":[0.0007109179,0.00012324053,0.00022819945,0.0007557981,0.00067879114,0.0003363257,0.00055994093,0.0004143815,0.00024072523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011479597,0.0004393947,0.5639587,0.00008756497,0.00009481928,0.0032487193,0.0014508817,0.01603547,0.37307215,0.0058832676,0.00064344547,0.033937637],"study_design_scores_gemma":[0.00027090995,0.0010940382,0.7935761,0.00003269099,0.000115265924,0.0022304517,0.0026886838,0.09681321,0.09240289,0.007306387,0.0033367793,0.00013260524],"about_ca_topic_score_codex":0.012502944,"about_ca_topic_score_gemma":0.010842238,"teacher_disagreement_score":0.012502944,"about_ca_system_score_codex":0.000547645,"about_ca_system_score_gemma":0.00036442484,"threshold_uncertainty_score":0.024860322},"labels":[],"label_agreement":null},{"id":"W2081260751","doi":"10.1086/376410","title":"Canonical Extra Mixing in Low‐Mass Red Giants","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Globular cluster; Red-giant branch; Mixing (physics); Astrophysics; Stars; Stellar evolution; Metallicity; Horizontal branch; Astronomy","score_opus":0.012563258083901819,"score_gpt":0.2294304618652104,"score_spread":0.21686720378130858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081260751","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999172,0.00007281458,0.00046508585,0.0000084657395,9.727465e-7,8.213587e-7,0.00003531421,0.0000159948,0.00022852824],"genre_scores_gemma":[0.9994405,0.00003429677,0.00034871203,0.0000060026205,0.0000018047456,8.9080703e-7,0.00008093228,0.00000430103,0.00008253867],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999012,0.000014987111,0.0000070820033,0.00003703909,0.000015869813,0.00002395057],"domain_scores_gemma":[0.9995652,0.00006695305,0.00017758472,0.00005614125,0.000040652936,0.00009351768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026793306,0.00019475371,0.00019043277,0.0005613035,0.00026896552,0.00057874445,0.00022801374,0.00021268263,0.00053885084],"category_scores_gemma":[0.0007154233,0.00016990949,0.00024822322,0.0004382661,0.00030192986,0.00048080314,0.00074661395,0.00024011712,0.00011889234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050475716,0.000023090783,0.89442587,0.000060476774,0.00009193919,0.00055057084,0.00067052344,0.0057636914,0.078208245,0.0029893026,0.00009751473,0.01661396],"study_design_scores_gemma":[0.00001941934,0.00010104127,0.9618119,0.000010900558,0.00006286096,0.0007539328,0.00015906061,0.017667849,0.014376763,0.0035391985,0.0014691012,0.000027996723],"about_ca_topic_score_codex":0.0022027441,"about_ca_topic_score_gemma":0.002680843,"teacher_disagreement_score":0.0022027441,"about_ca_system_score_codex":0.00042942946,"about_ca_system_score_gemma":0.0001367531,"threshold_uncertainty_score":0.0043798685},"labels":[],"label_agreement":null},{"id":"W2081304718","doi":"10.1088/0004-637x/706/1/727","title":"DISTRIBUTION AND CHARACTERISTICS OF INFRARED DARK CLOUDS USING GENETIC FORWARD MODELLING","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Milky Way; Molecular cloud; Extinction (optical mineralogy); Stars; Galaxy; Spiral galaxy; Infrared; Mass distribution; Population; Star formation; Interstellar medium; Astronomy","score_opus":0.013405988050630554,"score_gpt":0.23621416313580687,"score_spread":0.2228081750851763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081304718","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98539126,0.00003373819,0.013169445,0.000025426367,0.0000020486334,0.000017355538,0.0004488098,0.00009956335,0.0008124455],"genre_scores_gemma":[0.99069947,0.000029728519,0.007794308,0.0000046384916,0.0000020908576,0.000010353582,0.0011494406,0.000024044002,0.00028595026],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997986,0.000053781143,0.0000106073085,0.00006308302,0.000044698445,0.000029313649],"domain_scores_gemma":[0.9983399,0.0008700481,0.00030854341,0.0001636658,0.00021485107,0.00010295452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007718572,0.00034056537,0.00023928043,0.0016895673,0.00037983147,0.0008304303,0.0005405165,0.00032785517,0.00070681],"category_scores_gemma":[0.0033938794,0.0001557612,0.00056182756,0.0012995611,0.00028662608,0.00031209944,0.00034698192,0.00026449317,0.000249066],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002229593,0.00009311405,0.6833863,0.000027871945,0.00013982647,0.00041125552,0.00034312977,0.27558246,0.008328509,0.0025574407,0.00039292363,0.028514197],"study_design_scores_gemma":[0.000010952755,0.000030244642,0.13683003,0.000008790258,0.00003236046,0.0001978843,0.00009923553,0.8586827,0.0018743603,0.001624445,0.00058561837,0.000023369908],"about_ca_topic_score_codex":0.024561407,"about_ca_topic_score_gemma":0.01150758,"teacher_disagreement_score":0.024561407,"about_ca_system_score_codex":0.00086078583,"about_ca_system_score_gemma":0.0003847534,"threshold_uncertainty_score":0.048836887},"labels":[],"label_agreement":null},{"id":"W2081560085","doi":"10.1086/321472","title":"Galaxy Spin Statistics and Spin‐Density Correlation","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Galaxy; Physics; Weak gravitational lensing; Observable; Sky; Astrophysics; Spin (aerodynamics); Spin density; Statistical physics; Quantum mechanics; Redshift","score_opus":0.007199802463749494,"score_gpt":0.22170363293906084,"score_spread":0.21450383047531135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081560085","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3805705,0.0035769693,0.5597839,0.0036498015,0.00016403638,0.00006064637,0.0009362878,0.0007256535,0.050532166],"genre_scores_gemma":[0.98370034,0.0016909154,0.010457228,0.00011840639,0.00034040035,0.000065285916,0.00034818106,0.00007973756,0.0031995452],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99964285,0.0001376248,0.0000145791755,0.000053518856,0.00008196615,0.000069495734],"domain_scores_gemma":[0.99357116,0.004056622,0.0008732421,0.00067477825,0.00060018594,0.00022402235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017397004,0.000448165,0.00046905587,0.0027075282,0.0005852381,0.0015909343,0.00084152224,0.0005240344,0.0034449545],"category_scores_gemma":[0.010968957,0.0002591728,0.00033395272,0.001996823,0.002161535,0.0022845794,0.0010508067,0.0006980501,0.0007734479],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000015799036,0.000016966162,0.0062212767,0.000027269405,0.000012484201,0.00005779951,0.00007005357,0.042369794,0.00040734556,0.9389899,0.002009883,0.009801396],"study_design_scores_gemma":[0.000005345347,0.0000185685,0.0049198912,0.000032334232,0.000012421489,0.0001600005,0.000038324717,0.37312627,0.00049380824,0.6188563,0.002310711,0.000025913138],"about_ca_topic_score_codex":0.0022734413,"about_ca_topic_score_gemma":0.0011295618,"teacher_disagreement_score":0.0034449545,"about_ca_system_score_codex":0.0013348833,"about_ca_system_score_gemma":0.00055457,"threshold_uncertainty_score":0.011524498},"labels":[],"label_agreement":null},{"id":"W2081579166","doi":"10.1088/0004-637x/779/2/101","title":"PERIODIC OPTICAL VARIABILITY OF RADIO-DETECTED ULTRACOOL DWARFS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Semtech (Canada)","funders":"","keywords":"Astrophysics; Physics; Brown dwarf; Rotation period; Astronomy; Stellar classification; Stars","score_opus":0.006718766743198447,"score_gpt":0.20576369203234535,"score_spread":0.1990449252891469,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081579166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992188,0.000066260895,0.00015412235,0.0000041546054,0.0000015805826,0.000001623317,0.00012316366,0.000010926528,0.00041931547],"genre_scores_gemma":[0.99938655,0.00003323315,0.00020769236,0.0000060669486,0.000004223989,0.0000021234384,0.00023386089,0.000003308479,0.00012308569],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999045,0.000009537875,0.000008000413,0.000034041805,0.00002234932,0.000021607915],"domain_scores_gemma":[0.9995328,0.000049530874,0.0002397027,0.000036077807,0.000064634085,0.00007727561],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018048416,0.00009713522,0.00013059596,0.0008295434,0.00019188852,0.00034817797,0.00015623735,0.00010001955,0.00033718706],"category_scores_gemma":[0.00039899547,0.000066811575,0.000089302914,0.00043435488,0.00019947752,0.00013573456,0.0002874331,0.000101869395,0.00012921383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009338781,0.000017922835,0.9645176,0.000022460941,0.000022367509,0.0001338076,0.00029347232,0.00014352996,0.026738739,0.000052977703,0.000097195705,0.007866645],"study_design_scores_gemma":[0.0000010911149,0.000023684264,0.9983773,0.0000027337132,0.000006078117,0.00013255139,0.00008526535,0.00016778515,0.0009570199,0.000018995957,0.00022598855,0.0000015141379],"about_ca_topic_score_codex":0.0020219993,"about_ca_topic_score_gemma":0.003691767,"teacher_disagreement_score":0.0020219993,"about_ca_system_score_codex":0.0001804155,"about_ca_system_score_gemma":0.00007548171,"threshold_uncertainty_score":0.004020512},"labels":[],"label_agreement":null},{"id":"W2081713255","doi":"10.1086/429691","title":"Evidence of an Untruncated Accretion Disk in the Broad-Line Radio Galaxy 4C 74.26","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; RADIUS; Accretion (finance); Accretion disc; Black hole (networking); Line (geometry); Schwarzschild radius; Galaxy; Astronomy; Intermediate polar; Active galactic nucleus; Circular orbit; Quasar; Stars; Geometry; White dwarf","score_opus":0.02559101188842598,"score_gpt":0.27228792660110823,"score_spread":0.24669691471268226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081713255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985788,0.00015755878,0.000094479976,0.00002607948,0.000006792814,0.0000029910268,0.00004369537,0.00001601405,0.0010736157],"genre_scores_gemma":[0.99903107,0.00008928078,0.00028444873,0.000038543043,0.000016001712,0.0000038765825,0.00011663469,0.0000055621967,0.00041451704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998728,0.000008895591,0.000005003131,0.000026525893,0.000031924887,0.000054853328],"domain_scores_gemma":[0.9994311,0.00004116806,0.00024406453,0.00007376612,0.0000615543,0.0001481938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001591037,0.00041735696,0.0002494453,0.0010366254,0.0008314327,0.00074320764,0.0008079631,0.00045808556,0.001519407],"category_scores_gemma":[0.00050846615,0.00029138062,0.000121849276,0.00050973555,0.0012730167,0.00031847708,0.0007135644,0.00027707385,0.0005670492],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000628165,0.0002659793,0.68535507,0.00012551912,0.0001131128,0.0053640236,0.0007277328,0.00144968,0.28262237,0.0021775747,0.0015216281,0.019649213],"study_design_scores_gemma":[0.00004538466,0.00018079381,0.99099547,0.000015208567,0.000049232924,0.0014146841,0.00018593002,0.0007033296,0.003741579,0.00035216488,0.00229044,0.000025774603],"about_ca_topic_score_codex":0.0069140033,"about_ca_topic_score_gemma":0.011372888,"teacher_disagreement_score":0.0069140033,"about_ca_system_score_codex":0.0006397286,"about_ca_system_score_gemma":0.00022962666,"threshold_uncertainty_score":0.013747513},"labels":[],"label_agreement":null},{"id":"W2081943772","doi":"10.1088/0004-637x/762/1/8","title":"MESA MODELS OF CLASSICAL NOVA OUTBURSTS: THE MULTICYCLE EVOLUTION AND EFFECTS OF CONVECTIVE BOUNDARY MIXING","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; TRIUMF","funders":"","keywords":"White dwarf; Physics; Astrophysics; Nova (rocket); Accretion (finance); Convection; Stellar evolution; Dwarf nova; Mixing (physics); Stars; Mechanics","score_opus":0.014048042969151861,"score_gpt":0.2396732076135116,"score_spread":0.22562516464435975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081943772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9825801,0.00019393749,0.011334401,0.0001559015,0.000025552685,0.000029922958,0.00032666008,0.000119553,0.0052339905],"genre_scores_gemma":[0.994836,0.00009566604,0.0034580866,0.00003348076,0.000013356901,0.000038738406,0.00020818248,0.00004055571,0.0012758902],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999175,0.000026497444,0.0000053289596,0.000016048385,0.000011331449,0.000023273296],"domain_scores_gemma":[0.9991829,0.00035431772,0.00015723877,0.000076177384,0.000057160312,0.00017218599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034975287,0.00053162925,0.00049474,0.0004756797,0.0005287575,0.00088878337,0.00091317826,0.00076100806,0.001598442],"category_scores_gemma":[0.0018730867,0.00036757626,0.00070510345,0.00027712298,0.00068247394,0.00070253725,0.0009165398,0.0005371371,0.0001535255],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022208344,0.00010185307,0.015500598,0.000034904777,0.00005452239,0.00023268908,0.00008989033,0.96579826,0.0026731482,0.012858979,0.0004550794,0.001977958],"study_design_scores_gemma":[0.000025072828,0.000014805262,0.0015851035,0.0000027946244,0.0000049669607,0.000023993001,0.000014328665,0.9957475,0.00023417754,0.0021612758,0.00018144675,0.000004577813],"about_ca_topic_score_codex":0.008179642,"about_ca_topic_score_gemma":0.0064148684,"teacher_disagreement_score":0.008179642,"about_ca_system_score_codex":0.0007713906,"about_ca_system_score_gemma":0.00038715047,"threshold_uncertainty_score":0.016264021},"labels":[],"label_agreement":null},{"id":"W2081977449","doi":"10.1086/521395","title":"Dynamics of Dense Cores in the Perseus Molecular Cloud","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Molecular cloud; Dynamics (music); Cloud computing; Atmospheric dynamics; Gas dynamics; Computational astrophysics; Orbital mechanics","score_opus":0.006982030391254955,"score_gpt":0.2422868578913319,"score_spread":0.23530482750007695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2081977449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99494714,0.00011638766,0.000094051844,0.00030448975,0.000043337204,0.000008599261,0.000121691926,0.000021812335,0.004342607],"genre_scores_gemma":[0.9981048,0.00005193519,0.00005547855,0.000027084334,0.000019066098,0.0000020182754,0.000103366256,0.000004755174,0.0016315505],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999959,0.0000038892226,0.0000013364921,0.000009584853,0.000013372806,0.000012858736],"domain_scores_gemma":[0.9994505,0.000098591656,0.000093088674,0.000019936917,0.00015076705,0.00018714726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014553525,0.000109923945,0.00017673368,0.0003195705,0.00037550586,0.00056492747,0.00021722006,0.00019973428,0.0047969013],"category_scores_gemma":[0.0012753656,0.00009171771,0.000065396816,0.00017306756,0.00021746334,0.00023921838,0.00042127783,0.00016027449,0.00046621053],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001905994,0.00042289653,0.68669116,0.00021416477,0.0001424641,0.0040593515,0.0014218157,0.09043794,0.07991183,0.018890148,0.039309274,0.07659311],"study_design_scores_gemma":[0.00032362054,0.0002811947,0.82072353,0.000038968872,0.0000441491,0.00032470364,0.000990447,0.15197858,0.009218705,0.0054696035,0.010575877,0.000030617346],"about_ca_topic_score_codex":0.012408483,"about_ca_topic_score_gemma":0.011713123,"teacher_disagreement_score":0.012408483,"about_ca_system_score_codex":0.0006218066,"about_ca_system_score_gemma":0.00039186486,"threshold_uncertainty_score":0.024672568},"labels":[],"label_agreement":null},{"id":"W2082026304","doi":"10.1088/0004-637x/690/1/102","title":"NATURE AND NURTURE IN DARK MATTER HALOS","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Halo; Dark matter; Astrophysics; Substructure; Accretion (finance); Relaxation (psychology); Instability; Nature versus nurture; Astronomy; Galaxy; Quantum mechanics; Biology; Neuroscience","score_opus":0.0042482987532784415,"score_gpt":0.19708019428672965,"score_spread":0.1928318955334512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082026304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97726715,0.00040983365,0.010620772,0.0006738118,0.000017126682,0.000013107061,0.00005259892,0.00012685209,0.010818835],"genre_scores_gemma":[0.9980597,0.00011322856,0.001150207,0.000025880374,0.000005895207,0.000004821766,0.000019909327,0.000016127953,0.00060420274],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998809,0.00006224906,0.0000045450506,0.000015673033,0.00001643582,0.000020158628],"domain_scores_gemma":[0.9989604,0.0005066596,0.00016801094,0.00009920004,0.00005021832,0.00021550906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007671542,0.00018014098,0.0002645416,0.00042761044,0.00056484505,0.0010227881,0.00051654497,0.0005257108,0.0026365672],"category_scores_gemma":[0.004757595,0.00026964673,0.00034198325,0.00024065987,0.001451728,0.0017301916,0.0010480623,0.00044741845,0.0001882869],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033283213,0.00007757998,0.07299486,0.00017402325,0.000111110494,0.00062939594,0.0017999902,0.41622996,0.0067898147,0.48546657,0.0017796009,0.013614222],"study_design_scores_gemma":[0.00015770667,0.000106425,0.02904899,0.00003663436,0.0000539911,0.00034489512,0.00049509906,0.7096565,0.0019781424,0.25449467,0.0035823698,0.000044594704],"about_ca_topic_score_codex":0.0031447413,"about_ca_topic_score_gemma":0.0022266824,"teacher_disagreement_score":0.0031447413,"about_ca_system_score_codex":0.00078857504,"about_ca_system_score_gemma":0.00034537519,"threshold_uncertainty_score":0.008820236},"labels":[],"label_agreement":null},{"id":"W2082030684","doi":"10.1086/312652","title":"Strong Lensing Reconstruction","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Optical Polarization and Ellipsometry","field":"Engineering","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Smoothing; Weak gravitational lensing; Observable; Algorithm; Noise (video); Physics; Optics; Mathematics; Computer science; Image (mathematics); Astrophysics; Artificial intelligence; Statistics","score_opus":0.007574512149284737,"score_gpt":0.1975077876234986,"score_spread":0.18993327547421388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082030684","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0053572743,0.000049000046,0.99272305,0.00009332067,0.000012815382,0.000019921827,0.00012532675,0.00035010625,0.0012691992],"genre_scores_gemma":[0.125222,0.00016171814,0.86634094,0.000118098396,0.00006404533,0.00010222524,0.0006897894,0.00029089686,0.007010267],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995459,0.00009847448,0.000020942107,0.00011258662,0.0001664327,0.000055665838],"domain_scores_gemma":[0.99938345,0.0001661117,0.00007354036,0.00018497939,0.0001447508,0.000047231166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008668739,0.0009354762,0.00065941375,0.00079479057,0.00047546596,0.0013609553,0.0014151818,0.0010414763,0.0061881263],"category_scores_gemma":[0.0027563088,0.0005022867,0.00066893914,0.00071474153,0.0006638084,0.001382731,0.002642609,0.001234351,0.0028646854],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003793505,0.000077693316,0.0018453806,0.0002571831,0.00011740866,0.00023486254,0.00016984416,0.19957444,0.06363089,0.16747965,0.007075255,0.5591581],"study_design_scores_gemma":[0.00002518613,0.00004447026,0.00042694647,0.0000097726215,0.000015278432,0.00010476542,0.00003547995,0.92578876,0.018737193,0.04850381,0.0062826173,0.000025765825],"about_ca_topic_score_codex":0.0010145076,"about_ca_topic_score_gemma":0.0012955002,"teacher_disagreement_score":0.0061881263,"about_ca_system_score_codex":0.00042890946,"about_ca_system_score_gemma":0.00091978634,"threshold_uncertainty_score":0.020701349},"labels":[],"label_agreement":null},{"id":"W2082104851","doi":"10.1086/380557","title":"The Expansion of G11.2-0.3, a Radio Composite Supernova Remnant","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Supernova remnant; Supernova; Near-Earth supernova; Shell (structure); Measure (data warehouse)","score_opus":0.008019648723712396,"score_gpt":0.21470177767299467,"score_spread":0.20668212894928228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082104851","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994771,0.000040690313,0.00005865236,0.000003903941,0.000001266537,0.0000020237812,0.00013217589,0.000010625944,0.00027352167],"genre_scores_gemma":[0.998657,0.000041664644,0.0002459465,0.00000910276,0.000003414199,0.0000030855251,0.000836134,0.000006906429,0.00019682608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999596,0.0000030160181,0.0000025153388,0.000013887,0.0000076203705,0.000013429712],"domain_scores_gemma":[0.99970883,0.000030979336,0.000115639785,0.000033121305,0.00002408388,0.00008733878],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017759504,0.00021913137,0.00014134435,0.0007012639,0.00018203132,0.00036647145,0.00017131523,0.0001620302,0.00036714357],"category_scores_gemma":[0.000319238,0.000092372145,0.0001943015,0.00036772783,0.00020033677,0.00014029672,0.00025758587,0.00014967447,0.00021979112],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013556461,0.00011687024,0.87249005,0.00004401168,0.0000894204,0.0017718861,0.0002761333,0.0013444237,0.11108074,0.0005212362,0.0005095723,0.010400014],"study_design_scores_gemma":[0.000009457681,0.00008348798,0.99541986,0.0000024224469,0.000019318524,0.0011366352,0.000044735953,0.00054756727,0.0020966523,0.00005139098,0.0005830291,0.0000055766004],"about_ca_topic_score_codex":0.0054253917,"about_ca_topic_score_gemma":0.008194961,"teacher_disagreement_score":0.0054253917,"about_ca_system_score_codex":0.00032154046,"about_ca_system_score_gemma":0.00011824867,"threshold_uncertainty_score":0.010787606},"labels":[],"label_agreement":null},{"id":"W2082153469","doi":"10.1086/318406","title":"The Effect of the Cosmic Web on Cluster Weak Lensing Mass Estimates","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; St. Mary's University","funders":"","keywords":"Weak gravitational lensing; Physics; Cluster (spacecraft); Astrophysics; Structure formation; Dark matter; Galaxy cluster; Gravitational lensing formalism; Mass distribution; Line-of-sight; Galaxy; Strong gravitational lensing; Redshift; Computer science","score_opus":0.004986249821688269,"score_gpt":0.2118675887761539,"score_spread":0.20688133895446562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082153469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9654394,0.001339383,0.022108478,0.00083473587,0.000055366007,0.00003078469,0.00068043155,0.0004384018,0.0090731215],"genre_scores_gemma":[0.99632615,0.00016823466,0.0029243864,0.000046877118,0.000021822452,0.000007365342,0.00016195039,0.00005489006,0.00028828354],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9968183,0.0018600588,0.00012990733,0.00038129638,0.00066450454,0.00014595056],"domain_scores_gemma":[0.8943463,0.089243114,0.005811158,0.006385816,0.003361682,0.0008520086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0073431223,0.0006549865,0.00060257374,0.0021427812,0.00065531523,0.0017854127,0.0008292833,0.00086725724,0.0013573957],"category_scores_gemma":[0.09833426,0.000542046,0.00038493265,0.0015996181,0.0012604592,0.002608672,0.0019451486,0.0008991641,0.00035155605],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014846249,0.00009806699,0.49242815,0.00022382665,0.0006181107,0.0005235542,0.0003632345,0.42566612,0.0045024813,0.021058243,0.0020349498,0.050998617],"study_design_scores_gemma":[0.00009791525,0.0001364648,0.19394208,0.00011370875,0.00023820753,0.00034498624,0.00021220709,0.76667464,0.012136663,0.024103142,0.0018823525,0.0001176279],"about_ca_topic_score_codex":0.012345969,"about_ca_topic_score_gemma":0.008586245,"teacher_disagreement_score":0.012345969,"about_ca_system_score_codex":0.0012730295,"about_ca_system_score_gemma":0.00041042754,"threshold_uncertainty_score":0.03883463},"labels":[],"label_agreement":null},{"id":"W2082161920","doi":"10.1088/0004-637x/724/1/657","title":"SURFACE BRIGHTNESS FLUCTUATIONS IN THE<i>HUBBLE SPACE TELESCOPE</i>ACS/WFC F814W BANDPASS AND AN UPDATE ON GALAXY DISTANCES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Surface brightness; Galaxy; Fornax Cluster; Surface brightness fluctuation; Advanced Camera for Surveys; Virgo Cluster; Stellar population; Population; Astronomy; Galaxy cluster; Hubble space telescope; Star formation; Brightest cluster galaxy","score_opus":0.006210296023564818,"score_gpt":0.22759575222624165,"score_spread":0.22138545620267683,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082161920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898431,0.0005537146,0.0027774072,0.00010704508,0.000023138118,0.000015214632,0.002647563,0.0002082667,0.0038246207],"genre_scores_gemma":[0.9915696,0.00025272075,0.004493704,0.00004820528,0.000056586352,0.000012200181,0.0028961617,0.000039446717,0.0006312902],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960357,0.000036579575,0.00003077972,0.00012636291,0.00015144776,0.00005125359],"domain_scores_gemma":[0.9985959,0.00017656048,0.0005222083,0.00021851184,0.00039570118,0.00009110927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006388869,0.00034076493,0.00019115295,0.00195797,0.0003264009,0.00076487486,0.00035470017,0.0002950699,0.00056873227],"category_scores_gemma":[0.001528542,0.00018127805,0.00027024795,0.0012816088,0.00024505946,0.0005190307,0.00031882979,0.00026596643,0.000264414],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047235408,0.000020988069,0.9585751,0.000024161496,0.00004186035,0.000089049056,0.00015965929,0.0010767075,0.00914029,0.0002258975,0.0015425254,0.029056517],"study_design_scores_gemma":[7.2631303e-7,0.00001059268,0.9961695,0.0000041462267,0.000007863452,0.0000810134,0.000019946674,0.00097168627,0.0012633677,0.000032699118,0.0014321614,0.0000062497465],"about_ca_topic_score_codex":0.021329213,"about_ca_topic_score_gemma":0.028307935,"teacher_disagreement_score":0.021329213,"about_ca_system_score_codex":0.00063686946,"about_ca_system_score_gemma":0.00020295793,"threshold_uncertainty_score":0.042410135},"labels":[],"label_agreement":null},{"id":"W2082223380","doi":"10.1088/0004-637x/771/1/16","title":"AN IN-DEPTH VIEW OF THE MID-INFRARED PROPERTIES OF POINT SOURCES AND THE DIFFUSE ISM IN THE SMC GIANT H II REGION, N66","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Point source; Infrared; H II region; Supergiant; Ionization; Spectral line; Emission spectrum; Population; Interstellar medium","score_opus":0.012501694104429669,"score_gpt":0.21065783253680956,"score_spread":0.1981561384323799,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082223380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953015,0.0010203206,0.0004914508,0.000063130916,0.0000032426562,0.0000031362945,0.000103355786,0.0000069997177,0.0030069302],"genre_scores_gemma":[0.9975682,0.0007045522,0.0007734171,0.000040037026,0.000017899894,0.0000020318173,0.0001373397,0.0000026214652,0.0007538107],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996257,0.000003393935,0.0000020769633,0.000010085199,0.000011328405,0.000010650317],"domain_scores_gemma":[0.99992883,0.000008513135,0.000020947491,0.0000058777246,0.000011835706,0.00002398337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008289168,0.000120057,0.0001286824,0.000542627,0.00030656735,0.00036617144,0.0001690277,0.00022737634,0.0009762871],"category_scores_gemma":[0.000099714045,0.00007104623,0.00009267088,0.00035345645,0.00022092546,0.00038888122,0.00041802868,0.00020376261,0.00015981651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019748193,0.000060693088,0.6888628,0.00013372468,0.00002905681,0.00067532493,0.0013084384,0.000562039,0.28188193,0.0009065068,0.00023533535,0.025146704],"study_design_scores_gemma":[0.000001678332,0.000055418084,0.99524045,0.000008745082,0.000005579415,0.00036486943,0.0006358974,0.00035430506,0.0020593293,0.0001925939,0.0010775372,0.000003572896],"about_ca_topic_score_codex":0.0016786635,"about_ca_topic_score_gemma":0.006283256,"teacher_disagreement_score":0.0016786635,"about_ca_system_score_codex":0.00015013875,"about_ca_system_score_gemma":0.00007934032,"threshold_uncertainty_score":0.003337741},"labels":[],"label_agreement":null},{"id":"W2082231472","doi":"10.1086/430585","title":"<i>FUSE</i>Observations of the SMC 16 Day Wolf‐Rayet Binary Sanduleak 1 (WO4+O4): Atmospheric Eclipses and Colliding Stellar Winds","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Wolf–Rayet star; Radiative transfer; Stars; O-type star; Emission spectrum; Eclipse; Luminosity; Spectral line; Binary star; Astronomy; Galaxy","score_opus":0.014735676658584771,"score_gpt":0.21720773151097544,"score_spread":0.20247205485239067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082231472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987457,0.00005179096,0.00010984828,0.000008052663,0.00000243042,0.0000024478425,0.00047950525,0.000024190163,0.0005761303],"genre_scores_gemma":[0.99751943,0.000041410323,0.0004948438,0.000007847391,0.000008112152,0.0000035597045,0.0016013898,0.000007846231,0.00031559562],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992716,0.00000602229,0.0000045651705,0.000015636851,0.00002235392,0.000024260342],"domain_scores_gemma":[0.9998305,0.000015804231,0.00007381889,0.000017688355,0.000022500933,0.000039658167],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001468673,0.00019792814,0.00019343566,0.0011194033,0.00034710663,0.00033522514,0.00017303572,0.0002959052,0.0006220153],"category_scores_gemma":[0.00024138234,0.000106469575,0.0001833984,0.00051220885,0.00011168503,0.00017627052,0.00027823885,0.00015189045,0.00017380712],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005754064,0.00009905983,0.9017437,0.000054760367,0.00014276849,0.00078105554,0.00039066392,0.0028098605,0.076622024,0.00016650929,0.0008301133,0.015784115],"study_design_scores_gemma":[0.000008257875,0.000058092406,0.9914004,0.000006266457,0.000037890815,0.00017909394,0.00007802516,0.0027127904,0.00412831,0.00004565813,0.0013371323,0.000008029649],"about_ca_topic_score_codex":0.008158016,"about_ca_topic_score_gemma":0.019762004,"teacher_disagreement_score":0.008158016,"about_ca_system_score_codex":0.00036025126,"about_ca_system_score_gemma":0.000095610274,"threshold_uncertainty_score":0.016221106},"labels":[],"label_agreement":null},{"id":"W2082254641","doi":"10.1086/421769","title":"Quantitative Studies of the Far‐Ultraviolet, Ultraviolet, and Optical Spectra of Late O‐ and Early B‐Type Supergiants in the Magellanic Clouds","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supergiant; Astrophysics; Physics; Ultraviolet; Astronomy; Balmer series; Spectroscopy; Blanketing; Atmosphere (unit); Spectral line; Emission spectrum; Stars","score_opus":0.019404392708703793,"score_gpt":0.26401695851231655,"score_spread":0.24461256580361276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082254641","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988481,0.000071074275,0.00017325561,0.000002681412,5.623022e-7,0.0000019304975,0.00024455687,0.0000070380574,0.00065072963],"genre_scores_gemma":[0.99882215,0.000059434282,0.00033161163,0.0000054219804,0.0000036654324,0.0000034868926,0.00050109316,0.000003580813,0.00026961992],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992645,0.0000068652685,0.000004149162,0.00002726996,0.000016879903,0.000018343104],"domain_scores_gemma":[0.9996898,0.00006270167,0.00011021942,0.00001947818,0.00003570382,0.0000819822],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015635836,0.0002568705,0.000085337626,0.0014198485,0.0003059113,0.00025781436,0.00015734322,0.00015190711,0.00084912794],"category_scores_gemma":[0.0003034501,0.000080433565,0.00016010676,0.00078367064,0.00021344099,0.0003104616,0.00024551715,0.0001527047,0.0001760844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021902546,0.000055365523,0.85596746,0.00006903485,0.000053274118,0.00013647307,0.0008163083,0.0007003572,0.13047,0.00025865063,0.00011731259,0.011136627],"study_design_scores_gemma":[0.0000010126267,0.000038519705,0.9975345,0.000001302742,0.000005037122,0.00008321915,0.00008341915,0.00022415623,0.0018152336,0.00003402012,0.0001773007,0.0000021781398],"about_ca_topic_score_codex":0.0021946589,"about_ca_topic_score_gemma":0.003467817,"teacher_disagreement_score":0.0021946589,"about_ca_system_score_codex":0.00017350212,"about_ca_system_score_gemma":0.000044598444,"threshold_uncertainty_score":0.0043637156},"labels":[],"label_agreement":null},{"id":"W2082597868","doi":"10.1086/498562","title":"The Effect of Pre–Main‐Sequence Stars on Star Cluster Dynamics","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Stars; Sequence (biology); Physics; Cluster (spacecraft); Star (game theory); Star cluster; Blue straggler; Astrophysics; Pseudorandom binary sequence; Main sequence; Binary number; Mathematics; Chemistry; Computer science","score_opus":0.004934475830950985,"score_gpt":0.21861511937167039,"score_spread":0.2136806435407194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082597868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99499595,0.00034710934,0.0012130423,0.00020351176,0.00007998737,0.00003105041,0.00033058273,0.00014253771,0.002656183],"genre_scores_gemma":[0.99773264,0.00021337475,0.0011171979,0.00008472669,0.000017756225,0.00002048582,0.00023481992,0.000063342486,0.0005156856],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99961567,0.00011327602,0.000024991508,0.0000713842,0.00005536566,0.00011915131],"domain_scores_gemma":[0.9944137,0.0035775304,0.00037942044,0.00034213866,0.00051762053,0.0007695401],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009359185,0.00088763447,0.0007902782,0.00046339602,0.000903001,0.0013581889,0.0015386555,0.0013082587,0.0034293549],"category_scores_gemma":[0.009309124,0.00055514544,0.00070770644,0.0005643236,0.00075222226,0.0010807574,0.0010454796,0.0015096385,0.0003194517],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020473727,0.0007080618,0.040732328,0.00034034773,0.0002780851,0.00050053594,0.00026603125,0.9224772,0.02113512,0.0032148443,0.00087301683,0.0074271145],"study_design_scores_gemma":[0.0005690795,0.0019419829,0.03041029,0.00009687585,0.0003237434,0.0001561708,0.00035720554,0.93807423,0.02307579,0.001811791,0.0030732886,0.000109573266],"about_ca_topic_score_codex":0.011748902,"about_ca_topic_score_gemma":0.010897705,"teacher_disagreement_score":0.011748902,"about_ca_system_score_codex":0.0009817039,"about_ca_system_score_gemma":0.0012259679,"threshold_uncertainty_score":0.023361027},"labels":[],"label_agreement":null},{"id":"W2082598434","doi":"10.1088/0004-637x/691/1/705","title":"ACTIVE GALACTIC NUCLEUS HOST GALAXY MORPHOLOGIES IN COSMOS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Bulge; Active galactic nucleus; Redshift; Astronomy; Surface brightness; Asymmetry; Galaxy formation and evolution","score_opus":0.008958554966244094,"score_gpt":0.22509314498204114,"score_spread":0.21613459001579705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082598434","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96291256,0.00018887407,0.0021999232,0.000037312155,0.000020607558,0.000047608784,0.017206952,0.00067174056,0.016714416],"genre_scores_gemma":[0.95623994,0.00018707005,0.0043334113,0.000042911535,0.00002028827,0.000065459804,0.035305407,0.00023293702,0.0035726805],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997669,0.000020221212,0.000017623484,0.00009996703,0.000062951985,0.000032407006],"domain_scores_gemma":[0.99952257,0.000041559182,0.00015610628,0.00011010486,0.00007893763,0.000090840105],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002513176,0.00036003202,0.00026093045,0.0025810774,0.00022187752,0.0010611553,0.0002668801,0.0001307688,0.0061806],"category_scores_gemma":[0.0008735745,0.00016863266,0.00027425325,0.0018698438,0.00018521534,0.00042455038,0.0007131273,0.00021607918,0.0020127036],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013697584,0.00007373496,0.96198994,0.000041600742,0.0001331583,0.00013437058,0.00036118575,0.0024442687,0.005307077,0.0020226745,0.006596213,0.020758767],"study_design_scores_gemma":[0.00001158946,0.00002035294,0.9842084,0.000011933653,0.000016294483,0.00020809394,0.00014426268,0.0032502406,0.0010619757,0.00045886493,0.010594594,0.00001331643],"about_ca_topic_score_codex":0.0073151323,"about_ca_topic_score_gemma":0.008383834,"teacher_disagreement_score":0.0073151323,"about_ca_system_score_codex":0.00035477238,"about_ca_system_score_gemma":0.00011185172,"threshold_uncertainty_score":0.020676196},"labels":[],"label_agreement":null},{"id":"W2082638927","doi":"10.1088/0004-637x/738/1/63","title":"SPIDER OPTIMIZATION. II. OPTICAL, MAGNETIC, AND FOREGROUND EFFECTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Cosmic microwave background; Spider; Polarization (electrochemistry); Gravitational wave; Magnetic field; Amplitude; Detector; Cosmic background radiation; Microwave","score_opus":0.00799143923654122,"score_gpt":0.2179056866034244,"score_spread":0.2099142473668832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082638927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.66075283,0.0014124989,0.23832993,0.0010433341,0.00014492203,0.00039805644,0.0040488616,0.005768918,0.08810057],"genre_scores_gemma":[0.87264663,0.00023442484,0.11729918,0.0003812621,0.0000210639,0.00023619544,0.0019755382,0.00096631073,0.006239474],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9997447,0.000078902034,0.0000107467795,0.000043915174,0.00006280236,0.00005889145],"domain_scores_gemma":[0.9993599,0.0003072039,0.000049595186,0.000111639405,0.00013211554,0.00003958412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006078129,0.0007039896,0.0006868587,0.00045508397,0.00038188885,0.00077933446,0.00062521826,0.0007549569,0.0054449425],"category_scores_gemma":[0.0026761438,0.00031300532,0.00045781204,0.0005174172,0.00033077653,0.0007791322,0.0007221981,0.0005658587,0.0010487355],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066949526,0.00024064344,0.012986595,0.0002860422,0.00022334722,0.00019476289,0.00012359026,0.8569246,0.008874262,0.010032861,0.011214186,0.098229684],"study_design_scores_gemma":[0.00014108841,0.00018193225,0.0032475148,0.000027753194,0.000058459413,0.00011100325,0.00010376919,0.9766174,0.0057949056,0.0056079947,0.008083503,0.000024627465],"about_ca_topic_score_codex":0.0040159635,"about_ca_topic_score_gemma":0.006428118,"teacher_disagreement_score":0.0054449425,"about_ca_system_score_codex":0.00059244904,"about_ca_system_score_gemma":0.0010721061,"threshold_uncertainty_score":0.01821518},"labels":[],"label_agreement":null},{"id":"W2082674267","doi":"10.1088/0004-637x/779/1/32","title":"HerMES: THE CONTRIBUTION TO THE COSMIC INFRARED BACKGROUND FROM GALAXIES SELECTED BY MASS AND REDSHIFT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Redshift; Infrared; Star formation; Stellar mass; Astronomy","score_opus":0.005108716276243841,"score_gpt":0.19640998764598677,"score_spread":0.19130127136974293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082674267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98029774,0.00063297927,0.0027777203,0.00007458507,0.00002188391,0.000023405375,0.008529377,0.00049516,0.0071472116],"genre_scores_gemma":[0.98418415,0.00028146684,0.0010305482,0.00003386118,0.000056077002,0.000022046397,0.0128117865,0.00006379738,0.0015162646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990445,0.00019364413,0.00003821521,0.00025606257,0.00029878106,0.00016876447],"domain_scores_gemma":[0.998588,0.00030526696,0.00037748035,0.00028922883,0.00021310418,0.00022689973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008605271,0.0005406497,0.00042713745,0.0031069221,0.00020013194,0.0009202987,0.0004380015,0.00016577537,0.0022887199],"category_scores_gemma":[0.002441694,0.0001792495,0.0003309882,0.001912624,0.00020755967,0.00043302387,0.0008214794,0.00019014064,0.0006463111],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002961098,0.000039575432,0.95821774,0.000062819985,0.00030135136,0.00010824621,0.0002376352,0.0014636329,0.005654646,0.001434,0.0020320397,0.030152347],"study_design_scores_gemma":[0.000006245464,0.000023761637,0.9932774,0.000008329807,0.000037525606,0.0000933442,0.00006581466,0.0022466527,0.0011936218,0.00031583625,0.0027238205,0.000007688796],"about_ca_topic_score_codex":0.0049235267,"about_ca_topic_score_gemma":0.0063265925,"teacher_disagreement_score":0.0049235267,"about_ca_system_score_codex":0.00038155643,"about_ca_system_score_gemma":0.00014572481,"threshold_uncertainty_score":0.009789705},"labels":[],"label_agreement":null},{"id":"W2082782158","doi":"10.1086/424691","title":"Andromeda IX: A New Dwarf Spheroidal Satellite of M31","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Andromeda; Physics; Astrophysics; Photometry (optics); Dwarf spheroidal galaxy; Andromeda Galaxy; Astronomy; Sky; Local Group; Galaxy; Dwarf galaxy; Surface brightness; Red-giant branch; Milky Way; Globular cluster; Interacting galaxy; Stars","score_opus":0.007960084061629206,"score_gpt":0.21119481206636967,"score_spread":0.20323472800474046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082782158","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97980714,0.0037511569,0.0021105397,0.00036469277,0.00014624832,0.00005674788,0.00066324725,0.00019327621,0.012906992],"genre_scores_gemma":[0.98902065,0.0009462091,0.004655273,0.0001561525,0.000116657844,0.000021971828,0.0020692153,0.000020353884,0.0029936335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982893,0.000013069164,0.0000067905726,0.00006708974,0.000049614962,0.00003449916],"domain_scores_gemma":[0.999617,0.000030227626,0.00010132574,0.00006878034,0.00004313179,0.0001395708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028654712,0.00027019848,0.00024163978,0.0005200429,0.0007085709,0.00070476695,0.00039087542,0.00039385652,0.0014876887],"category_scores_gemma":[0.0003993897,0.00015446894,0.00020154574,0.0004474792,0.00037041097,0.0006191732,0.0008451326,0.0004869558,0.0009383784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012075785,0.00026745818,0.5600616,0.0005648076,0.00016051823,0.0064040925,0.0031612285,0.0020291668,0.28117836,0.016417593,0.010743812,0.117803864],"study_design_scores_gemma":[0.00012339397,0.0013668522,0.6269958,0.00015798307,0.00010237438,0.018911084,0.00094411825,0.0044295853,0.028892044,0.0050636344,0.3128978,0.00011537175],"about_ca_topic_score_codex":0.0010861622,"about_ca_topic_score_gemma":0.0015221048,"teacher_disagreement_score":0.0014876887,"about_ca_system_score_codex":0.00031603413,"about_ca_system_score_gemma":0.000281113,"threshold_uncertainty_score":0.0049768686},"labels":[],"label_agreement":null},{"id":"W2082789373","doi":"10.1088/0004-637x/760/2/149","title":"<i>SPITZER</i>AND<i>HERSCHEL</i>MULTIWAVELENGTH CHARACTERIZATION OF THE DUST CONTENT OF EVOLVED H II REGIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; H II region; Cosmic dust; Galaxy; Star formation","score_opus":0.022188268474261794,"score_gpt":0.22439215653874164,"score_spread":0.20220388806447986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082789373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918836,0.000041412015,0.0002779146,0.0000040236073,4.4479015e-7,0.0000014290625,0.00033403322,0.000013582745,0.0001387897],"genre_scores_gemma":[0.99768186,0.000028835731,0.00082017883,0.0000068890076,0.000004085753,0.000003883698,0.0013122284,0.000010418472,0.00013165454],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998808,0.000015986847,0.000007300671,0.000048091606,0.0000199055,0.000027947604],"domain_scores_gemma":[0.9996687,0.00004259443,0.00012649002,0.00006473257,0.000045046992,0.000052465046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029945472,0.00025085555,0.00018868677,0.0010709459,0.00019606017,0.0003341174,0.00030256668,0.0001589651,0.0005000639],"category_scores_gemma":[0.00038301785,0.00015172499,0.0003248701,0.00055446004,0.00020663594,0.00024244127,0.00027166956,0.0001447758,0.00013006655],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000099221535,0.00003658796,0.93507487,0.000021867805,0.00013456345,0.00014030574,0.0001391028,0.0050655226,0.053914048,0.00014728056,0.000110652145,0.0051159672],"study_design_scores_gemma":[0.0000030847555,0.000011449655,0.99539787,0.0000011103848,0.0000109263165,0.00004991831,0.000021100046,0.0016701838,0.0026258484,0.000030286314,0.0001743359,0.000003904672],"about_ca_topic_score_codex":0.002706708,"about_ca_topic_score_gemma":0.0044319723,"teacher_disagreement_score":0.002706708,"about_ca_system_score_codex":0.00029480923,"about_ca_system_score_gemma":0.00007612752,"threshold_uncertainty_score":0.005381882},"labels":[],"label_agreement":null},{"id":"W2082791406","doi":"10.1088/0004-637x/738/2/144","title":"THE STELLAR ARCHEOLOGY OF THE M33 DISK: RECENT STAR-FORMING HISTORY AND CONSTRAINTS ON THE TIMING OF AN INTERACTION WITH M31,","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Local Group; Star formation; RADIUS; Stars; Galaxy formation and evolution; Hubble sequence; Effective radius","score_opus":0.0228276700332952,"score_gpt":0.21453209160978634,"score_spread":0.19170442157649115,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082791406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983504,0.00015060297,0.00008638987,0.000017304772,8.9103276e-7,0.000002668268,0.00030349902,0.00000921651,0.0010790514],"genre_scores_gemma":[0.99917454,0.00006894279,0.00021776072,0.000004813623,0.0000018018613,0.0000014759306,0.00036528052,0.0000022468325,0.00016319545],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997866,0.0000018741498,0.0000011618741,0.000005287747,0.0000066148677,0.00000637475],"domain_scores_gemma":[0.9998271,0.0000145943,0.000075602,0.000019369481,0.000022891756,0.000040470077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007321615,0.000076195574,0.00005539429,0.00075527065,0.00019239676,0.00022088228,0.000113297676,0.00019399422,0.0009476557],"category_scores_gemma":[0.00028496506,0.00007395582,0.000086788416,0.0006012325,0.00014622562,0.00018678878,0.000184164,0.00013257565,0.0002417133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024902375,0.00003893689,0.8679645,0.00010257282,0.000035159075,0.00053251773,0.0009435812,0.00049025094,0.10607903,0.00046864085,0.000980928,0.02211494],"study_design_scores_gemma":[9.705218e-7,0.000017751427,0.9984243,0.0000031812535,0.0000029242424,0.00016719404,0.000056069257,0.00022563933,0.0005667297,0.000020741747,0.000513626,9.642217e-7],"about_ca_topic_score_codex":0.006681075,"about_ca_topic_score_gemma":0.023774644,"teacher_disagreement_score":0.006681075,"about_ca_system_score_codex":0.00029803487,"about_ca_system_score_gemma":0.00011230465,"threshold_uncertainty_score":0.013284385},"labels":[],"label_agreement":null},{"id":"W2082871840","doi":"10.1086/498738","title":"The Spatial Distribution of Metals in the Intergalactic Medium","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Metallicity; Quasar; Galaxy; Intergalactic travel; Intergalactic medium; Line (geometry); Absorption (acoustics); Lyman limit","score_opus":0.005166394956334374,"score_gpt":0.20899409881608252,"score_spread":0.20382770385974816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082871840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991541,0.00009619413,0.00008538794,0.000011748453,4.2670584e-7,5.9664194e-7,0.00010739749,0.000004711203,0.0005393319],"genre_scores_gemma":[0.9996294,0.00005305088,0.00006731422,0.0000032679693,0.0000021853157,6.0498127e-7,0.00012881405,0.0000017959517,0.000113530004],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998702,0.00002063423,0.000006021488,0.000042709842,0.000024895213,0.000035448622],"domain_scores_gemma":[0.9991466,0.00021855853,0.0003052339,0.00007352427,0.00010363294,0.00015242618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014988771,0.00012820278,0.00021298583,0.001499515,0.00019077041,0.0009770972,0.0002759271,0.00021301568,0.0012554373],"category_scores_gemma":[0.0007652296,0.00013093337,0.00009629395,0.0016523054,0.00034037887,0.0005146521,0.00084750314,0.00013742171,0.00033859088],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013290557,0.000021490636,0.982496,0.000013920515,0.000055702934,0.00021810576,0.00031072393,0.0008404225,0.009284474,0.0005363401,0.00009398217,0.005995928],"study_design_scores_gemma":[0.0000035767232,0.000023244182,0.9974112,0.000002426043,0.000012558623,0.00013655724,0.00030826696,0.0009479968,0.0005721685,0.00021417762,0.00036308804,0.000004694802],"about_ca_topic_score_codex":0.0031838634,"about_ca_topic_score_gemma":0.0047562355,"teacher_disagreement_score":0.0031838634,"about_ca_system_score_codex":0.00030662463,"about_ca_system_score_gemma":0.00007582988,"threshold_uncertainty_score":0.006330669},"labels":[],"label_agreement":null},{"id":"W2082889578","doi":"10.1088/0004-637x/790/2/129","title":"PHYSICAL AND CHEMICAL CHARACTERISTICS OF L1689-SMM16, AN OSCILLATING PRESTELLAR CORE IN OPHIUCHUS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; National Research Council Canada; University of Victoria","funders":"","keywords":"Ophiuchus; Physics; Astrophysics; Protostar; Molecular cloud; Core (optical fiber); Virial mass; Star formation; Astronomy; Virial theorem; Stars; Galaxy","score_opus":0.01218515140290173,"score_gpt":0.2459889003507207,"score_spread":0.233803748947819,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082889578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99977094,0.00002269945,0.00001403614,0.0000030938402,5.2563814e-7,0.0000015363047,0.000056314708,0.0000022305803,0.00012869365],"genre_scores_gemma":[0.99936205,0.000019370724,0.00010924151,0.000007679795,0.0000024476858,0.0000036124259,0.0003129519,0.0000028023276,0.00017981858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999659,0.0000018354177,0.0000027545266,0.000012684459,0.000008182215,0.000008638014],"domain_scores_gemma":[0.9998355,0.000006833357,0.000056406876,0.000006613901,0.000016153752,0.000078497505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000050316834,0.00021295028,0.00021356069,0.0005807143,0.00025043447,0.00017453269,0.00023233036,0.00021840734,0.0006307064],"category_scores_gemma":[0.00014180024,0.00011962298,0.00011374723,0.00023471315,0.00020405483,0.00013252471,0.0003399025,0.00014408596,0.00025012498],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054182933,0.000098341996,0.6817385,0.00003953554,0.000035638444,0.0009124412,0.00039076596,0.00036473168,0.30933794,0.00006803725,0.00016633849,0.00630596],"study_design_scores_gemma":[0.000008328276,0.000099319484,0.9971451,0.0000030166239,0.000004194299,0.00034317074,0.00012245306,0.0002901582,0.0017103145,0.000022278655,0.00024753067,0.000004156574],"about_ca_topic_score_codex":0.004933608,"about_ca_topic_score_gemma":0.006936007,"teacher_disagreement_score":0.004933608,"about_ca_system_score_codex":0.00029504826,"about_ca_system_score_gemma":0.00008961514,"threshold_uncertainty_score":0.009809732},"labels":[],"label_agreement":null},{"id":"W2082947388","doi":"10.1086/527561","title":"A Massive-Star-forming Infrared Loop around the Crab-like Supernova Remnant G54.1+0.3: Post-Main-Sequence Triggered Star Formation?","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Stars; Young stellar object; Supernova; Spitzer Space Telescope; Star formation; Astronomy; Supernova remnant; Infrared; RADIUS","score_opus":0.018834697511721406,"score_gpt":0.2584111543774711,"score_spread":0.2395764568657497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082947388","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99883527,0.00023615304,0.00036718484,0.000057662885,0.000010010794,0.0000067042715,0.000046652807,0.000022920618,0.0004174756],"genre_scores_gemma":[0.99913245,0.00007471353,0.0004184394,0.000067114976,0.00001740029,0.0000024463443,0.00011083533,0.0000025367892,0.00017404482],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999341,0.000004060529,0.000004294987,0.000022499404,0.000010238101,0.00002477206],"domain_scores_gemma":[0.99978703,0.000014051125,0.00011001463,0.000023495193,0.000011540771,0.000053880165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013930586,0.000246704,0.00024487777,0.00027114866,0.00032786018,0.0005411578,0.00043807313,0.00057718495,0.00079066836],"category_scores_gemma":[0.00028744267,0.0001346806,0.00022132944,0.0001718448,0.00033243085,0.000223718,0.00042492186,0.00027154293,0.00030588591],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009452225,0.00017023899,0.814361,0.000088446934,0.000094998366,0.035343613,0.00038580102,0.0002796429,0.13220589,0.0009450572,0.0006840776,0.014496011],"study_design_scores_gemma":[0.000086420805,0.0012989042,0.8690738,0.000033530192,0.00021304422,0.09036671,0.000657717,0.0031372418,0.027942196,0.0010057265,0.006144032,0.000040566934],"about_ca_topic_score_codex":0.0008822902,"about_ca_topic_score_gemma":0.001200241,"teacher_disagreement_score":0.0008822902,"about_ca_system_score_codex":0.00019717318,"about_ca_system_score_gemma":0.00009744676,"threshold_uncertainty_score":0.0026450157},"labels":[],"label_agreement":null},{"id":"W2082993322","doi":"10.1088/0004-637x/744/1/6","title":"SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC). IV. A CENSUS OF VERY LOW MASS OBJECTS IN NGC 1333","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Physics; Stars; Stellar classification; Astrophysics; RADIUS; Low Mass; Astronomy; Population; Cluster (spacecraft)","score_opus":0.012982019031189887,"score_gpt":0.2168169977228055,"score_spread":0.2038349786916156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2082993322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939003,0.00017310069,0.0003225661,0.0000227701,0.000002734478,0.00001854757,0.004786774,0.00005325715,0.0007200479],"genre_scores_gemma":[0.98343974,0.00018242767,0.0015831464,0.000028689432,0.000008838421,0.000034760033,0.014011534,0.000024366083,0.0006865341],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998368,0.0000096792355,0.000011661209,0.000044071607,0.000047716847,0.000050091883],"domain_scores_gemma":[0.9994311,0.00003064987,0.00018780443,0.00004905417,0.00008637244,0.00021503339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018616718,0.00019677839,0.00023918257,0.0018918107,0.0007100215,0.000519144,0.00030035994,0.00017969239,0.0018691898],"category_scores_gemma":[0.00031036217,0.00009907003,0.0002495578,0.0023243243,0.0002335735,0.00024453804,0.000737437,0.00023997841,0.0005782681],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016217792,0.00003934975,0.9636615,0.00004351423,0.000029823808,0.00024184198,0.00052877126,0.0002751128,0.017434573,0.00025645047,0.0020745713,0.015252312],"study_design_scores_gemma":[0.0000017862144,0.000016238568,0.997959,0.000003042028,0.000005194491,0.00016031723,0.00010175573,0.00019856644,0.00042367828,0.00002925748,0.001098195,0.0000030145231],"about_ca_topic_score_codex":0.033893067,"about_ca_topic_score_gemma":0.06627368,"teacher_disagreement_score":0.033893067,"about_ca_system_score_codex":0.0004794021,"about_ca_system_score_gemma":0.0004650745,"threshold_uncertainty_score":0.067391574},"labels":[],"label_agreement":null},{"id":"W2083299008","doi":"10.1086/375524","title":"The G11.11-0.12 Infrared-dark Cloud: Anomalous Dust and a Nonmagnetic Isothermal Model","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Protein filament; Infrared; Cosmic dust; Galaxy; Molecular cloud; Interstellar medium; Absorption (acoustics); Interstellar cloud; Extinction (optical mineralogy); Astronomy; Materials science; Optics; Stars","score_opus":0.007834083444339482,"score_gpt":0.21184293975028343,"score_spread":0.20400885630594395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083299008","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94315135,0.0006340015,0.019705817,0.001489893,0.0000912047,0.00009819799,0.00068665354,0.00027506656,0.03386793],"genre_scores_gemma":[0.99461323,0.00014664618,0.0010581983,0.00007384094,0.0000742052,0.000022039228,0.00018694277,0.000023005176,0.0038017507],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998673,0.000018917257,0.000004555886,0.0000238603,0.000018682727,0.00006658404],"domain_scores_gemma":[0.9995233,0.00006029767,0.00010094955,0.00003501576,0.000044077457,0.0002364034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003018038,0.00053564546,0.000543146,0.00063756906,0.0008831368,0.0010539477,0.001931791,0.00091998925,0.0030688199],"category_scores_gemma":[0.0006196024,0.00027940213,0.0006458988,0.00036094067,0.0012450443,0.0010032103,0.0007299244,0.00044487667,0.00064445136],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012460258,0.0005362562,0.10509119,0.00015711949,0.00013494836,0.0028086493,0.00076005346,0.4326108,0.016538002,0.41831782,0.007788468,0.014010615],"study_design_scores_gemma":[0.00031405865,0.000116005285,0.035597585,0.000019065095,0.000050796876,0.00048974913,0.00014514248,0.890496,0.00039907807,0.06960243,0.0027177983,0.000052261857],"about_ca_topic_score_codex":0.03424559,"about_ca_topic_score_gemma":0.0152342785,"teacher_disagreement_score":0.03424559,"about_ca_system_score_codex":0.0012963358,"about_ca_system_score_gemma":0.00065626996,"threshold_uncertainty_score":0.068092525},"labels":[],"label_agreement":null},{"id":"W2083374520","doi":"10.1088/0004-637x/755/2/161","title":"CALCIUM-RICH GAP TRANSIENTS IN THE REMOTE OUTSKIRTS OF GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":224,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Galaxy; Astrophysics; Astronomy; Red shift","score_opus":0.019923303489746393,"score_gpt":0.24931883747452713,"score_spread":0.22939553398478074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083374520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99936026,0.000052418556,0.00002347381,0.000009219474,9.183885e-7,0.0000024913086,0.000112392045,0.0000058949904,0.0004328874],"genre_scores_gemma":[0.9994634,0.000038208673,0.00004264807,0.000010401106,0.0000044604544,0.000001981978,0.00031652683,0.0000027488973,0.00011959659],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987686,0.000006597814,0.0000077701,0.00005022247,0.000018458783,0.000040055547],"domain_scores_gemma":[0.99943227,0.00005241973,0.00024100639,0.000032851076,0.00003328996,0.00020811884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016330782,0.0001959527,0.00026649237,0.002061455,0.0004682131,0.0009194547,0.0002848708,0.00029275395,0.0015053957],"category_scores_gemma":[0.0005224414,0.00013945963,0.00018004156,0.00075950735,0.00037702586,0.0003723419,0.0008416493,0.00024582562,0.00028831934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000871453,0.000024390452,0.99267805,0.000008096319,0.00001552947,0.0002777036,0.00033256997,0.00004424179,0.0039011366,0.00010925008,0.00009476282,0.0024271696],"study_design_scores_gemma":[0.0000018446042,0.000013615412,0.9994579,0.0000020183495,0.0000031645898,0.00015754177,0.00013381927,0.000042403044,0.00006497086,0.000022183085,0.00009958024,0.0000010119576],"about_ca_topic_score_codex":0.008357355,"about_ca_topic_score_gemma":0.0154549815,"teacher_disagreement_score":0.008357355,"about_ca_system_score_codex":0.00033595524,"about_ca_system_score_gemma":0.00014625714,"threshold_uncertainty_score":0.016617417},"labels":[],"label_agreement":null},{"id":"W2083390656","doi":"10.1086/322463","title":"Temporal and Spectral Characteristics of Short Bursts from the Soft Gamma Repeaters 1806−20 and 1900+14","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Fluence; Gamma-ray burst; Magnetar; Log-normal distribution; Spectral line; Light curve; Spectral properties; Spectral slope","score_opus":0.012243141278397192,"score_gpt":0.2810634499974138,"score_spread":0.2688203087190166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083390656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989322,0.00006461212,0.00018093083,0.000009463702,0.0000013585084,0.000003044321,0.00025360996,0.00002107492,0.00053374114],"genre_scores_gemma":[0.9978042,0.000060805953,0.00030282195,0.000007867265,0.0000116996425,0.0000070009414,0.0015247385,0.000015560676,0.00026535607],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999926,0.000005885348,0.0000065637514,0.000018910356,0.00002257242,0.000020162284],"domain_scores_gemma":[0.99897635,0.00022183746,0.0005173516,0.00005728885,0.00008858207,0.00013858515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014748746,0.00017531325,0.00015556127,0.0013998023,0.00017431282,0.00028025213,0.00018762417,0.00016513314,0.0008940818],"category_scores_gemma":[0.0008688925,0.00011141709,0.00015870959,0.0009379262,0.0001904135,0.00015358494,0.00028216664,0.00015716959,0.0002745324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007989288,0.00009809711,0.91155356,0.000066166256,0.00008871604,0.0005364583,0.0005160365,0.0015498188,0.060322057,0.00044355902,0.00045850474,0.023568153],"study_design_scores_gemma":[0.0000060647376,0.00005609829,0.9972842,0.0000024964704,0.000011055652,0.00035684288,0.000047186328,0.0007943527,0.0010363874,0.00007477023,0.00032470716,0.00000577408],"about_ca_topic_score_codex":0.0013559258,"about_ca_topic_score_gemma":0.002514692,"teacher_disagreement_score":0.0013998023,"about_ca_system_score_codex":0.00016179461,"about_ca_system_score_gemma":0.000057742218,"threshold_uncertainty_score":0.002990961},"labels":[],"label_agreement":null},{"id":"W2083405175","doi":"10.1088/0004-637x/786/2/84","title":"TIMING AND FLUX EVOLUTION OF THE GALACTIC CENTER MAGNETAR SGR J1745–2900","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Magnetar; Galactic Center; Flux (metallurgy); Astrophysics; Astronomy; Center (category theory); Neutron star; Galaxy","score_opus":0.008758372892418131,"score_gpt":0.2724922930602392,"score_spread":0.26373392016782105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083405175","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983461,0.00009371234,0.00010501822,0.000025033163,0.0000057664197,0.0000027074907,0.0006660868,0.000021685255,0.0007338946],"genre_scores_gemma":[0.9977715,0.000042545882,0.00021655594,0.000013500069,0.000009391586,0.0000026504333,0.0016393781,0.0000057482366,0.0002987791],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999404,0.0000047510107,0.000004018257,0.000020454794,0.000015543212,0.000014792871],"domain_scores_gemma":[0.9996038,0.00003790451,0.00019088988,0.000022157714,0.00006275591,0.00008249259],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014650194,0.00019163036,0.0001495388,0.0011732174,0.00019255091,0.0003548116,0.00019443197,0.00024020733,0.00091972493],"category_scores_gemma":[0.00046079274,0.000082317914,0.00014452229,0.0005445311,0.00016474012,0.0001614394,0.00024646608,0.00017883364,0.00019773497],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034237653,0.000085334206,0.94114065,0.00004901738,0.00008098929,0.00055530225,0.0002878695,0.0015924599,0.0404684,0.00034763073,0.0012599623,0.013789948],"study_design_scores_gemma":[0.0000023375726,0.00003334313,0.9982438,0.0000026782875,0.0000069135335,0.00010072768,0.000030107125,0.00045782208,0.0006585738,0.000015128494,0.0004455258,0.0000030225522],"about_ca_topic_score_codex":0.009310914,"about_ca_topic_score_gemma":0.015492445,"teacher_disagreement_score":0.009310914,"about_ca_system_score_codex":0.0003657146,"about_ca_system_score_gemma":0.000109120396,"threshold_uncertainty_score":0.018513441},"labels":[],"label_agreement":null},{"id":"W2083413347","doi":"10.1088/0004-637x/732/1/3","title":"DIRECT CONFIRMATION OF THE ASYMMETRY OF THE CAS A SUPERNOVA WITH LIGHT ECHOES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Supernova; Asymmetry; Spectral line; Spectroscopy; H-alpha; Connection (principal bundle); Outflow; Optical spectra","score_opus":0.011175012568748794,"score_gpt":0.2029780657109325,"score_spread":0.1918030531421837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083413347","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9795989,0.00045286078,0.0030597546,0.0002507813,0.00020338545,0.000042198968,0.0005846696,0.00010691607,0.015700605],"genre_scores_gemma":[0.9974031,0.00008493296,0.0008362668,0.00005509821,0.000029254792,0.000013365353,0.00027192105,0.000016889542,0.0012891741],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9996704,0.00006032886,0.000032119962,0.00009880651,0.000065172484,0.00007314943],"domain_scores_gemma":[0.99774086,0.000438095,0.00042643753,0.0006535276,0.0003485278,0.00039263372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006582619,0.00029485056,0.00020785972,0.0014418997,0.0006522431,0.0008206278,0.00040005214,0.0006500695,0.007836405],"category_scores_gemma":[0.0026347772,0.00014643198,0.00028487897,0.00077877846,0.0010288561,0.00038350504,0.0011145603,0.0007312448,0.00064128987],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0034337486,0.00033259648,0.33631557,0.0002217629,0.00029971145,0.00907288,0.00073600694,0.00057261647,0.57574743,0.025465023,0.0027714404,0.045031168],"study_design_scores_gemma":[0.00032660252,0.0012374682,0.73216575,0.000097328826,0.0003508581,0.054672074,0.0021476746,0.005194863,0.15254347,0.015817199,0.035325572,0.00012123644],"about_ca_topic_score_codex":0.0014469767,"about_ca_topic_score_gemma":0.0011199223,"teacher_disagreement_score":0.007836405,"about_ca_system_score_codex":0.0002194929,"about_ca_system_score_gemma":0.0003724894,"threshold_uncertainty_score":0.026215374},"labels":[],"label_agreement":null},{"id":"W2083477024","doi":"10.1088/0004-637x/694/2/1131","title":"DWARF GALAXY CLUSTERING AND MISSING SATELLITES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics","funders":"","keywords":"Dwarf galaxy; Galaxy; Milky Way; Dwarf spheroidal galaxy; Redshift; Interacting galaxy; Satellite galaxy; Dwarf galaxy problem; Stellar mass","score_opus":0.008584018149295377,"score_gpt":0.21864818207902914,"score_spread":0.21006416392973376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083477024","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864906,0.00014076197,0.0001773242,0.00004699018,0.0000012337431,0.0000012917819,0.00016830943,0.000012754283,0.00080244226],"genre_scores_gemma":[0.9995964,0.000017600058,0.000065269785,0.000004876572,0.0000018889122,4.8494394e-7,0.00014893927,0.0000016867615,0.00016273848],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997011,0.00004956596,0.000018065432,0.00009027428,0.000074918564,0.00006595117],"domain_scores_gemma":[0.99653435,0.0007435963,0.0014949117,0.00033537162,0.00034387034,0.00054777454],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003278408,0.00011257355,0.00022946995,0.0009901909,0.00029564014,0.00043347696,0.00027079653,0.00030404463,0.0014044784],"category_scores_gemma":[0.0027777164,0.00011327995,0.00015438502,0.0011247537,0.00036063837,0.00029324056,0.0004423464,0.00018513376,0.0002699199],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045468994,0.0000074723257,0.99447256,0.000008302485,0.000023339231,0.00009203613,0.00012508714,0.0009997799,0.0009631048,0.00028533238,0.00018659949,0.002790997],"study_design_scores_gemma":[9.07053e-7,0.000009624203,0.99798226,0.0000028447978,0.0000049504265,0.0001725319,0.000070828355,0.0012400015,0.00018334635,0.00016936287,0.0001601434,0.0000033206034],"about_ca_topic_score_codex":0.010406095,"about_ca_topic_score_gemma":0.015931042,"teacher_disagreement_score":0.010406095,"about_ca_system_score_codex":0.0005430132,"about_ca_system_score_gemma":0.00018468998,"threshold_uncertainty_score":0.020691097},"labels":[],"label_agreement":null},{"id":"W2083481765","doi":"10.1088/0004-637x/693/2/1713","title":"OPTICAL SPECTROSCOPY OF X-RAY SOURCES IN THE EXTENDED CHANDRA DEEP FIELD SOUTH","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Harvard University; Carnegie Institution of Washington; Massachusetts Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Luminosity; Chandra Deep Field South; Spectrograph; Active galactic nucleus; Integral field spectrograph; Flux (metallurgy); Astronomy; Hubble Deep Field; Spectroscopy; Spectral line","score_opus":0.005882726356617144,"score_gpt":0.21801205122358952,"score_spread":0.21212932486697236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083481765","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966698,0.00032832418,0.000560286,0.000038398808,0.0000066053835,0.000018861114,0.00106067,0.000036889334,0.0012800836],"genre_scores_gemma":[0.99092287,0.00039407008,0.0046736887,0.00007247194,0.000046857625,0.000026492264,0.0029987823,0.000027003547,0.00083772605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978894,0.00001993302,0.000013261574,0.000056028806,0.00006565184,0.00005617524],"domain_scores_gemma":[0.9989967,0.00009346208,0.0003173987,0.00014190155,0.00018451674,0.00026613142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052550994,0.000383262,0.00038824408,0.0023126912,0.0005311949,0.0004857021,0.0003210369,0.00014306465,0.00113691],"category_scores_gemma":[0.00067743694,0.00033151874,0.00025306997,0.0013157385,0.00024700293,0.00040231337,0.001034482,0.00031238075,0.00029380474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005825304,0.00018700489,0.90141743,0.00016416631,0.00020128374,0.00041411546,0.0007756239,0.00038413637,0.06458793,0.00056569435,0.0015033667,0.029216647],"study_design_scores_gemma":[0.000019894884,0.00006554555,0.9951544,0.000009325345,0.0000344987,0.00032098917,0.00009407296,0.00020087566,0.0022663053,0.00012412964,0.0016983106,0.000011718554],"about_ca_topic_score_codex":0.00394001,"about_ca_topic_score_gemma":0.01040692,"teacher_disagreement_score":0.00394001,"about_ca_system_score_codex":0.00026581105,"about_ca_system_score_gemma":0.00028529996,"threshold_uncertainty_score":0.0078341365},"labels":[],"label_agreement":null},{"id":"W2083574565","doi":"10.1086/312702","title":"A Comparison of Estimators for the Two-Point Correlation Function","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Scientific Research and Discoveries","field":"Physics and Astronomy","cited_by":232,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Estimator; Statistics; Mathematics; Gaussian; Correlation; Variance (accounting); Function (biology); Correlation function (quantum field theory); Statistical physics; Computer science; Physics; Spectral density","score_opus":0.02269627717512996,"score_gpt":0.32479328702948107,"score_spread":0.3020970098543511,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083574565","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34696764,0.006233005,0.6406512,0.00040564197,0.0002210321,0.0001684305,0.0010577596,0.0010608429,0.0032343483],"genre_scores_gemma":[0.8114255,0.0017730446,0.18233743,0.0001046762,0.00017996611,0.00019073671,0.002878369,0.00033679153,0.0007733653],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99020445,0.005971075,0.0006575459,0.0011585645,0.0016215098,0.00038684244],"domain_scores_gemma":[0.8929404,0.085587434,0.0050634486,0.008823453,0.0065571214,0.0010281012],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.03062068,0.0008107542,0.0011054892,0.005031466,0.00054187316,0.0019200075,0.0017239625,0.0017317068,0.0010626308],"category_scores_gemma":[0.11200679,0.00037603124,0.00083193876,0.0023447848,0.0012223725,0.0028095199,0.0019612676,0.0009972118,0.0005062316],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024181225,0.00035586106,0.2655428,0.0015096592,0.00225226,0.0002587715,0.00091475825,0.15242292,0.008113632,0.0866411,0.0059443703,0.4736257],"study_design_scores_gemma":[0.0004146605,0.0025838926,0.20179732,0.00057240005,0.00072467816,0.0014118078,0.00083203387,0.70204175,0.019365504,0.05959125,0.010069319,0.0005953751],"about_ca_topic_score_codex":0.0011604346,"about_ca_topic_score_gemma":0.0011819274,"teacher_disagreement_score":0.03062068,"about_ca_system_score_codex":0.0007892637,"about_ca_system_score_gemma":0.0011076138,"threshold_uncertainty_score":0.16193956},"labels":[],"label_agreement":null},{"id":"W2083575068","doi":"10.1088/0004-637x/773/2/99","title":"HOT ELECTROMAGNETIC OUTFLOWS. II. JET BREAKOUT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Lorentz factor; Scattering; Lorentz force; Magnetic field; Jet (fluid); Photon; Forward scatter; Magnetization; Compton scattering; Radiation","score_opus":0.0065343652323110665,"score_gpt":0.20681720410346233,"score_spread":0.20028283887115125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083575068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84881216,0.0052926918,0.085086666,0.0006798699,0.00041772498,0.00017989875,0.00050662726,0.00035006134,0.058674283],"genre_scores_gemma":[0.9899005,0.000606808,0.002998807,0.00015606101,0.00016057098,0.000036602745,0.00016554457,0.00006677006,0.005908288],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986017,0.00002752123,0.000005042355,0.000027786087,0.000023924682,0.000055491706],"domain_scores_gemma":[0.9997905,0.00003474258,0.0000780255,0.000015419513,0.000019323203,0.000061981795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023698117,0.0008780659,0.0005726751,0.00052407756,0.0008796599,0.0014461358,0.00070364686,0.0010467182,0.0021031848],"category_scores_gemma":[0.0007614364,0.00032619032,0.00069358497,0.0003062019,0.0011919758,0.001049696,0.001120444,0.0007547055,0.00030065476],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075665145,0.00043396463,0.04830403,0.00045455317,0.00015026593,0.006205367,0.0005931771,0.60705584,0.05179769,0.25344658,0.002905372,0.027896505],"study_design_scores_gemma":[0.00028332043,0.0004110691,0.046611894,0.000087414555,0.00007885063,0.0016675727,0.00033785627,0.875403,0.0064164964,0.060286257,0.008338178,0.00007806187],"about_ca_topic_score_codex":0.0030610848,"about_ca_topic_score_gemma":0.0011437164,"teacher_disagreement_score":0.0030610848,"about_ca_system_score_codex":0.0009166355,"about_ca_system_score_gemma":0.00032336928,"threshold_uncertainty_score":0.0070358515},"labels":[],"label_agreement":null},{"id":"W2083708369","doi":"10.1088/0004-637x/714/1/163","title":"OBSERVATIONS OF THE SHELL-TYPE SUPERNOVA REMNANT CASSIOPEIA A AT TeV ENERGIES WITH VERITAS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cassiopeia A; Physics; Supernova remnant; Crab Nebula; Cherenkov radiation; Astrophysics; Flux (metallurgy); Telescope; Gamma ray; Astronomy; Near-Earth supernova; Photon; Supernova; Optics","score_opus":0.01232532805985222,"score_gpt":0.21045425554658673,"score_spread":0.1981289274867345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083708369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997598,0.0001625704,0.0002957186,0.000020156938,0.0000037940717,0.000007911629,0.0004481388,0.000054581855,0.0014090895],"genre_scores_gemma":[0.99617755,0.00020425326,0.0014519412,0.000014628712,0.000012555716,0.0000059213608,0.0014807124,0.000013178284,0.0006392899],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988055,0.000008341474,0.0000057856246,0.000038904032,0.000045891553,0.000020512369],"domain_scores_gemma":[0.99956626,0.000065052176,0.00013521883,0.00008303567,0.000077682686,0.0000726745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025666898,0.00021102668,0.00018291692,0.0007659573,0.00046217098,0.00041863002,0.00032986392,0.00020770617,0.0010118907],"category_scores_gemma":[0.0004405559,0.00019983467,0.00022906292,0.00058066484,0.0002715116,0.00026097972,0.0004801027,0.00029853167,0.0002247502],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007747684,0.00012754697,0.7673352,0.000107563166,0.00036699054,0.0027266117,0.00073027116,0.0017575121,0.2007303,0.0005174552,0.0016434517,0.023182405],"study_design_scores_gemma":[0.000021170512,0.0001857643,0.9857686,0.000010428598,0.00006844374,0.0010200606,0.000110244684,0.0009770143,0.009165679,0.000092013055,0.0025679488,0.000012593118],"about_ca_topic_score_codex":0.0090120565,"about_ca_topic_score_gemma":0.023148822,"teacher_disagreement_score":0.0090120565,"about_ca_system_score_codex":0.00038623146,"about_ca_system_score_gemma":0.00022590581,"threshold_uncertainty_score":0.017919183},"labels":[],"label_agreement":null},{"id":"W2083737225","doi":"10.1088/0004-637x/725/2/2392","title":"AN INFRARED NEBULA ASSOCIATED WITH δ CEPHEI: EVIDENCE OF MASS LOSS?","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Western University","funders":"","keywords":"Astrophysics; Physics; Nebula; Cepheid variable; Stars; Interstellar medium; Infrared; Proper motion; Astronomy; Bow shock (aerodynamics); Shock wave; Galaxy","score_opus":0.01076245881428053,"score_gpt":0.2502849199433943,"score_spread":0.23952246112911377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083737225","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984926,0.00021071403,0.00019603655,0.000044869383,0.0000073833567,0.0000038366793,0.000031838586,0.000008371148,0.0010043435],"genre_scores_gemma":[0.9995548,0.000055889966,0.0001574983,0.00002530673,0.000008971249,0.0000013006286,0.000030989722,7.9594895e-7,0.00016441596],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999622,0.0000021363649,0.0000016998833,0.000009888584,0.000009142655,0.000014899084],"domain_scores_gemma":[0.9998536,0.000023474204,0.000050489893,0.000016483216,0.000018533743,0.000037436617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009202381,0.00011982883,0.00014662466,0.000261617,0.00038016876,0.00036153608,0.00034273983,0.00031519518,0.0010955413],"category_scores_gemma":[0.00036434128,0.00008834495,0.00006506675,0.00018034257,0.00030230574,0.00019901285,0.00022609826,0.00027701704,0.0002483648],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056297885,0.00010434472,0.86916476,0.000059705137,0.000024194735,0.019137144,0.00052275206,0.00013704688,0.08541936,0.00068492343,0.0004733653,0.02370934],"study_design_scores_gemma":[0.000019259282,0.00033004335,0.93421334,0.000018839948,0.000031422038,0.052193075,0.0004920683,0.0007596896,0.007840825,0.0005259763,0.0035660597,0.000009488167],"about_ca_topic_score_codex":0.0014551114,"about_ca_topic_score_gemma":0.0017243121,"teacher_disagreement_score":0.0014551114,"about_ca_system_score_codex":0.00016187964,"about_ca_system_score_gemma":0.00007150849,"threshold_uncertainty_score":0.0036649108},"labels":[],"label_agreement":null},{"id":"W2083762031","doi":"10.1088/0004-637x/701/1/330","title":"THREE-DIMENSIONAL SIMULATIONS OF MAGNETIZED SUPERBUBBLES: NEW INSIGHTS INTO THE IMPORTANCE OF MHD EFFECTS ON OBSERVED QUANTITIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Magnetohydrodynamics; Superbubble; Physics; Magnetohydrodynamic drive; Magnetic field; Computational physics; Astrophysics; Lorentz force; Plane (geometry); Mechanics; Classical mechanics; Interstellar medium; Geometry; Galaxy; Mathematics","score_opus":0.013471688912516572,"score_gpt":0.2364453201138643,"score_spread":0.22297363120134772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083762031","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96081066,0.00037834703,0.024738368,0.0008160637,0.000063696214,0.000061077495,0.00051873695,0.0003104739,0.0123025905],"genre_scores_gemma":[0.99259186,0.00015935043,0.0057469816,0.00012032715,0.000024749868,0.000061494735,0.0002495796,0.000101158395,0.0009446443],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998429,0.00004303018,0.0000063893426,0.000017473863,0.000041563304,0.0000485845],"domain_scores_gemma":[0.998885,0.0005625786,0.00013645012,0.000065461056,0.00010155481,0.00024892832],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035922343,0.00051290845,0.0007718469,0.00041847583,0.00088173046,0.0013731145,0.0011717097,0.0014309033,0.002270836],"category_scores_gemma":[0.0021722328,0.00037070966,0.00058135233,0.00046938861,0.0010929165,0.0008725239,0.00096363685,0.001107204,0.00019847619],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010501809,0.00007410363,0.0037268542,0.000023827903,0.00003354807,0.0001431479,0.00013302981,0.98886263,0.0018824183,0.0037945693,0.0003482197,0.0008725158],"study_design_scores_gemma":[0.000029152221,0.000010573309,0.00068921165,0.0000033763333,0.0000040382915,0.000009402329,0.000025040163,0.99752396,0.00024337659,0.001220416,0.00023436881,0.000007063428],"about_ca_topic_score_codex":0.0179144,"about_ca_topic_score_gemma":0.007766659,"teacher_disagreement_score":0.0179144,"about_ca_system_score_codex":0.001242053,"about_ca_system_score_gemma":0.0007056641,"threshold_uncertainty_score":0.035620272},"labels":[],"label_agreement":null},{"id":"W2083772309","doi":"10.1086/427495","title":"The Intermediate‐Scale Clustering of Luminous Red Galaxies","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":212,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Astrophysics; Physics; Correlation function (quantum field theory); Galaxy; Redshift; Luminosity; Sky; Cluster analysis; Luminosity function; Astronomy; Statistics; Mathematics","score_opus":0.005930243882517879,"score_gpt":0.20638952441562652,"score_spread":0.20045928053310866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083772309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987571,0.00008991483,0.00023340844,0.000013285945,0.0000012764028,0.0000014551963,0.0003355307,0.000030015903,0.0005379415],"genre_scores_gemma":[0.99900275,0.000023531815,0.00021783545,0.000004781927,0.0000033889382,0.0000012893319,0.0006117082,0.000004319794,0.0001303733],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970657,0.000032811055,0.000012223097,0.000097019874,0.00006067089,0.00009067263],"domain_scores_gemma":[0.99879646,0.00011699662,0.0005417655,0.00014478006,0.000139167,0.00026083662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031741406,0.00018889594,0.00017255016,0.0013503206,0.00032082637,0.00047629152,0.00032809156,0.00017902405,0.0006589737],"category_scores_gemma":[0.0009466116,0.00014731092,0.00020912741,0.0009651171,0.00038414448,0.00021963149,0.0005965002,0.00024287158,0.00020624444],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000114808354,0.00002462925,0.9843203,0.000021458713,0.00008658391,0.00009921736,0.00028606216,0.001088994,0.00618661,0.00038265914,0.00057038834,0.006818306],"study_design_scores_gemma":[0.0000011416894,0.0000068864106,0.99910307,9.0544455e-7,0.000004150948,0.000032752123,0.000017895374,0.000392508,0.0002168797,0.00003553985,0.00018612284,0.0000022595254],"about_ca_topic_score_codex":0.012361165,"about_ca_topic_score_gemma":0.016473219,"teacher_disagreement_score":0.012361165,"about_ca_system_score_codex":0.00046896422,"about_ca_system_score_gemma":0.00014449391,"threshold_uncertainty_score":0.024578452},"labels":[],"label_agreement":null},{"id":"W2083853015","doi":"10.1088/0004-637x/774/1/5","title":"NEAR-INFRARED SPECTROSCOPY OF INFRARED-EXCESS STELLAR OBJECTS IN THE YOUNG SUPERNOVA REMNANT G54.1+0.3","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Supernova; Stars; Infrared; Stellar classification; RADIUS; Extinction (optical mineralogy); Spectral energy distribution; Spectral line; Astronomy; Absorption (acoustics); Spectroscopy; Infrared excess; Galaxy; Optics","score_opus":0.00921460923557766,"score_gpt":0.23475184647268743,"score_spread":0.22553723723710978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083853015","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99957424,0.00008181387,0.000078246,0.000006155516,0.0000014133135,0.0000022126176,0.0000574774,0.000009969336,0.00018855136],"genre_scores_gemma":[0.99856275,0.000083136765,0.00060713,0.000032744898,0.0000062613567,0.0000064984115,0.0005159758,0.0000055034034,0.00018002346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999237,0.0000064426226,0.000005326934,0.000024318078,0.000018554923,0.000021571677],"domain_scores_gemma":[0.9998111,0.000016164238,0.0000756984,0.000016337503,0.000022441907,0.000058311554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022980868,0.00025884144,0.00023372966,0.0006977588,0.00029639903,0.00027306037,0.00025167988,0.00027040645,0.00041924146],"category_scores_gemma":[0.00021263925,0.00012527502,0.0002527276,0.00032699393,0.0002212579,0.00014320387,0.00037404353,0.00018355604,0.00017591995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042496258,0.00011366944,0.5645257,0.00005083175,0.000109773864,0.00092507614,0.00035780555,0.00027756716,0.42604467,0.00021745842,0.00023745077,0.0067151343],"study_design_scores_gemma":[0.000012519138,0.00016335567,0.9924346,0.000004846928,0.000046449564,0.00067905267,0.00010809399,0.00029238954,0.0056702713,0.00005776256,0.00052322086,0.0000073094],"about_ca_topic_score_codex":0.0015975421,"about_ca_topic_score_gemma":0.002669218,"teacher_disagreement_score":0.0015975421,"about_ca_system_score_codex":0.00018555984,"about_ca_system_score_gemma":0.000060775244,"threshold_uncertainty_score":0.0031764507},"labels":[],"label_agreement":null},{"id":"W2083936836","doi":"10.1086/505695","title":"Atmospheres of Protoplanetary Cores: Critical Mass for Nucleated Instability","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":326,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Opacity; Physics; Astrophysics; Planet; Protoplanetary disk; Accretion (finance); Formation and evolution of the Solar System; Giant planet; Radiative transfer; Astronomy; Planetary migration; Planetary system","score_opus":0.010131380439687926,"score_gpt":0.24498069837499456,"score_spread":0.23484931793530664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2083936836","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973316,0.00019584055,0.0010526482,0.000049844577,0.000006168291,0.0000074867935,0.00007154356,0.000025958752,0.0012588708],"genre_scores_gemma":[0.99957615,0.000052226424,0.00017359834,0.000005380613,0.000006168927,0.0000039327133,0.000048209917,0.000005855006,0.00012846087],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994814,0.0000074845475,0.000001793905,0.000011877626,0.000009920201,0.00002084783],"domain_scores_gemma":[0.9995896,0.00012942965,0.00013132766,0.000016577425,0.000043932825,0.000089120775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001326003,0.0002237534,0.00017571641,0.00032647347,0.00040744568,0.00045239824,0.0003782719,0.00028254677,0.0006214082],"category_scores_gemma":[0.0011401002,0.0001648226,0.00028904813,0.00013023184,0.0004504051,0.00039136907,0.00030894863,0.00029017552,0.00005866764],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011181051,0.00042051362,0.24539094,0.00033746535,0.00029832465,0.002855281,0.00088709255,0.36773527,0.3266763,0.04117478,0.0020296967,0.011076164],"study_design_scores_gemma":[0.00013731362,0.00038063418,0.16474198,0.000024586172,0.00007483147,0.00063487055,0.00037328489,0.8013713,0.017694028,0.013146115,0.0013716684,0.000049435825],"about_ca_topic_score_codex":0.0027866024,"about_ca_topic_score_gemma":0.0012103162,"teacher_disagreement_score":0.0027866024,"about_ca_system_score_codex":0.0005224297,"about_ca_system_score_gemma":0.00026352107,"threshold_uncertainty_score":0.0055407286},"labels":[],"label_agreement":null},{"id":"W2084019993","doi":"10.1086/427409","title":"Erratum: “The<i>Swift</i>Gamma‐Ray Burst Mission” (ApJ, 611, 1005 [2004])","year":2005,"lang":"fr","type":"erratum","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Swift; Physics; Gamma-ray burst; Astrophysics; Astronomy","score_opus":0.015156940160418473,"score_gpt":0.27420107160701185,"score_spread":0.2590441314465934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084019993","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00059096335,0.0011563259,0.0004658791,0.043934792,0.93591654,0.000048183098,0.0043154466,0.00078101293,0.012790838],"genre_scores_gemma":[0.013752242,0.005298887,0.0040072775,0.099215925,0.16565053,0.00019134194,0.017535424,0.002456534,0.69189197],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9981369,0.00017607385,0.0003968805,0.0002263508,0.00088181364,0.00018203797],"domain_scores_gemma":[0.98925436,0.0011113179,0.0008136479,0.0007893038,0.0074718203,0.00055945525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019307506,0.0022334792,0.0016268758,0.0050633335,0.004904817,0.004295992,0.0025945813,0.005355086,0.06649998],"category_scores_gemma":[0.017587475,0.001010093,0.0016686678,0.0021421106,0.0012342476,0.0023385033,0.002037692,0.0052062306,0.05481507],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024032865,0.0000071033355,0.000054895532,0.000029199486,0.0000046778514,0.00006740132,0.000006519239,0.000014953756,0.000040892664,0.00017872019,0.997615,0.001956558],"study_design_scores_gemma":[0.00003798611,0.00003024998,0.002013437,0.00016311723,0.000041975516,0.00015550602,0.00006138847,0.00012720289,0.00048119633,0.000550194,0.99630415,0.0000334702],"about_ca_topic_score_codex":0.0428295,"about_ca_topic_score_gemma":0.057184037,"teacher_disagreement_score":0.06649998,"about_ca_system_score_codex":0.003879542,"about_ca_system_score_gemma":0.005006613,"threshold_uncertainty_score":0.22246456},"labels":[],"label_agreement":null},{"id":"W2084026462","doi":"10.1086/382747","title":"Gemini Imaging of QSO Host Galaxies at<i>z</i> ∼ 2","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"QSOS; Physics; Galaxy; Astrophysics; Redshift; Quasar; Stars; Active galactic nucleus; Astronomy; Star formation","score_opus":0.007085446859266182,"score_gpt":0.21397939425361479,"score_spread":0.2068939473943486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084026462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93291444,0.00075334613,0.0012739059,0.0015069703,0.00017215336,0.00004767269,0.0092802495,0.0012785308,0.052772783],"genre_scores_gemma":[0.9709226,0.00031215994,0.0020508678,0.00030771422,0.0002427358,0.000020663103,0.008704936,0.00020546392,0.017232973],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998392,0.000007974829,0.000005954915,0.00003854065,0.00004494725,0.000063350126],"domain_scores_gemma":[0.99944097,0.00004588883,0.00008182964,0.00007323831,0.00018961659,0.0001683337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040280362,0.00018461056,0.00022625654,0.0013377914,0.00065797154,0.0006871701,0.00026518834,0.0005251239,0.01591606],"category_scores_gemma":[0.00057925965,0.00023650151,0.00016401912,0.00086552114,0.00013752292,0.00059593,0.0003464055,0.0002590614,0.0022967325],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0030438174,0.00021351346,0.36332953,0.00038872604,0.00010911312,0.00146912,0.0011526411,0.00052519544,0.4520473,0.0027964956,0.08771564,0.087208964],"study_design_scores_gemma":[0.000059284455,0.000086774635,0.94631475,0.000023080096,0.00005481044,0.00047303637,0.00026035827,0.0010113611,0.024842305,0.0003414075,0.026515566,0.000017306169],"about_ca_topic_score_codex":0.0027663985,"about_ca_topic_score_gemma":0.0086117,"teacher_disagreement_score":0.01591606,"about_ca_system_score_codex":0.0003115266,"about_ca_system_score_gemma":0.00018688338,"threshold_uncertainty_score":0.05324447},"labels":[],"label_agreement":null},{"id":"W2084041236","doi":"10.1086/499239","title":"Mid-Infrared Emission from Elliptical Galaxies: Sensitivity to Stellar Age","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Balmer series; Elliptical galaxy; Galaxy; Stars; Spectral line; Stellar population; Stellar mass; Line (geometry)","score_opus":0.008346236560360012,"score_gpt":0.2179592937965446,"score_spread":0.2096130572361846,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084041236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970932,0.00037923746,0.0006766347,0.000034422745,0.000003881199,0.000006543072,0.00032084197,0.00004984179,0.0014352389],"genre_scores_gemma":[0.99840516,0.0001533966,0.000505244,0.00006949176,0.0000077991235,0.000006363487,0.0004938458,0.0000076128504,0.00035116347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969554,0.00004074371,0.000016730884,0.00012958009,0.00006272995,0.00005474745],"domain_scores_gemma":[0.9986773,0.0004273206,0.00037257827,0.00017023295,0.00017225636,0.00018015402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005345953,0.00016730318,0.00025186955,0.00047324086,0.000120373734,0.00047426127,0.0002853982,0.0004865969,0.0006934987],"category_scores_gemma":[0.0012316304,0.00025956155,0.0002731768,0.00024432526,0.0001836229,0.00036136262,0.00042747657,0.00027646084,0.00043408974],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018771713,0.000044357286,0.93828654,0.00003805585,0.000084348096,0.00005701723,0.00017641677,0.00073748117,0.04923055,0.00005496797,0.00018373942,0.01091875],"study_design_scores_gemma":[0.0000016201852,0.000018881115,0.99723405,0.000003033884,0.00001220479,0.00010733545,0.000018334758,0.00048303578,0.0018946927,0.00003113682,0.00019198771,0.0000037990083],"about_ca_topic_score_codex":0.0025592223,"about_ca_topic_score_gemma":0.0030742558,"teacher_disagreement_score":0.0025592223,"about_ca_system_score_codex":0.00024913962,"about_ca_system_score_gemma":0.000047068137,"threshold_uncertainty_score":0.005088687},"labels":[],"label_agreement":null},{"id":"W2084279698","doi":"10.1088/0004-637x/775/1/61","title":"HerMES: THE FAR-INFRARED EMISSION FROM DUST-OBSCURED GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Key Programme; Science and Technology Facilities Council; Centre National de la Recherche Scientifique; National Aeronautics and Space Administration; California Institute of Technology; Imperial College London; National Astronomical Observatories, Chinese Academy of Sciences; UK Space Agency; Centre National d’Etudes Spatiales; U.S. Department of Energy","keywords":"Astrophysics; Physics; Galaxy; Photometry (optics); Star formation; Active galactic nucleus; Far infrared; Luminous infrared galaxy; Luminosity; Infrared; Luminosity function; Spectral energy distribution; Astronomy; Population; Stars; Medicine","score_opus":0.007434381193018628,"score_gpt":0.2041971767174348,"score_spread":0.19676279552441617,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084279698","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9809771,0.00043920835,0.002097663,0.00003660703,0.000017807832,0.00002152702,0.0077097844,0.00042465486,0.008275739],"genre_scores_gemma":[0.98628104,0.00023545795,0.0022524484,0.000043133386,0.00005291525,0.00001465545,0.008711152,0.000050369585,0.002358779],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971884,0.00002824546,0.000009933619,0.0000848015,0.000087683,0.000070483635],"domain_scores_gemma":[0.9996425,0.000035716163,0.00013848065,0.000051628977,0.000029947912,0.000101715406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003417139,0.0003344976,0.0002808612,0.0017097392,0.00020592668,0.0006262109,0.00036635215,0.0001620387,0.0028427949],"category_scores_gemma":[0.0004240549,0.00017426479,0.00029637557,0.00097398675,0.00019523283,0.00034031284,0.0004907374,0.00013931569,0.00070472393],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017976602,0.00008846398,0.9435751,0.000116570955,0.0001794009,0.0003241821,0.00039818042,0.001229184,0.016659481,0.0014059251,0.0066169137,0.029226786],"study_design_scores_gemma":[0.0000060896623,0.000021712047,0.9930368,0.00000864806,0.000016151542,0.000179368,0.000069662536,0.00095897587,0.00096738944,0.00016267288,0.0045654317,0.0000071680374],"about_ca_topic_score_codex":0.0025545403,"about_ca_topic_score_gemma":0.0051196837,"teacher_disagreement_score":0.0028427949,"about_ca_system_score_codex":0.00018144853,"about_ca_system_score_gemma":0.00009061608,"threshold_uncertainty_score":0.00951004},"labels":[],"label_agreement":null},{"id":"W2084291270","doi":"10.1088/0004-637x/744/2/88","title":"TRACING THE STAR-FORMATION-DENSITY RELATION TO<i>z</i>∼ 2","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":149,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Star formation; Redshift; Galaxy; Cluster (spacecraft); Quenching (fluorescence); Galaxy cluster; Star cluster; Galaxy groups and clusters","score_opus":0.012989629952118434,"score_gpt":0.20242665330752868,"score_spread":0.18943702335541024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084291270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99531305,0.00011790395,0.0009975446,0.00006501577,0.0000020228247,0.000009151722,0.000753834,0.00007454477,0.0026668806],"genre_scores_gemma":[0.99792993,0.00004471022,0.00078311,0.000014045463,0.000003369317,0.0000071732966,0.0007944949,0.000012463984,0.00041079015],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983394,0.00002439675,0.000006962529,0.000061046725,0.000022452396,0.00005126012],"domain_scores_gemma":[0.99823785,0.00044989935,0.0006705722,0.00013196065,0.00029084898,0.00021891],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041469032,0.00020105975,0.00021666673,0.0019117367,0.00030891743,0.00076888985,0.00034426223,0.00039651888,0.0016621083],"category_scores_gemma":[0.002235682,0.00024166166,0.00022353376,0.0011575503,0.00037895603,0.00047839346,0.00069249416,0.00042131075,0.00054285384],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000093043614,0.000028533957,0.98280036,0.00002702239,0.000028332839,0.000080703816,0.0006063012,0.0014049234,0.00487433,0.0021691164,0.0004978423,0.007389608],"study_design_scores_gemma":[0.0000024188469,0.000011881514,0.9965307,0.000004542038,0.0000039950123,0.000045372864,0.00006711312,0.0017399644,0.0006054186,0.00031338554,0.0006713514,0.0000038747025],"about_ca_topic_score_codex":0.013248218,"about_ca_topic_score_gemma":0.017901855,"teacher_disagreement_score":0.013248218,"about_ca_system_score_codex":0.00064689654,"about_ca_system_score_gemma":0.00014704608,"threshold_uncertainty_score":0.026342213},"labels":[],"label_agreement":null},{"id":"W2084312993","doi":"10.1086/430299","title":"An Algorithm to Detect Blends with Eclipsing Binaries in Planet Transit Searches","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Victoria; University of Toronto","funders":"","keywords":"Transit (satellite); Planet; Stars; Exoplanet; Binary number; Eclipse; Gravitational lens; Planetary system; Residual","score_opus":0.012522144438343815,"score_gpt":0.2366326995331459,"score_spread":0.22411055509480207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084312993","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.042237185,0.00043495768,0.9379265,0.00025526865,0.00011279464,0.000591184,0.00086371216,0.014890293,0.0026881688],"genre_scores_gemma":[0.09726032,0.00011544248,0.8966756,0.00017421324,0.000064788685,0.00044149108,0.0024666854,0.0005297698,0.002271794],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99857116,0.00013089017,0.00017971756,0.00046494073,0.00047526255,0.00017802928],"domain_scores_gemma":[0.99818605,0.00047218482,0.00029145833,0.00029868525,0.0006131605,0.00013849612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011049834,0.0012269737,0.0010708465,0.0040030414,0.001436272,0.0022427198,0.002052917,0.0018509376,0.004063666],"category_scores_gemma":[0.00456988,0.00081371353,0.0011290412,0.0023046164,0.0006452835,0.001866823,0.0023607565,0.0013601733,0.0037543718],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006094532,0.0005547383,0.021718096,0.00022312511,0.00031275413,0.00057443534,0.00034722846,0.020288868,0.050467607,0.0028183248,0.0150760645,0.8870094],"study_design_scores_gemma":[0.00035963987,0.0004412272,0.016241329,0.00008721448,0.00023746907,0.0019787685,0.00049524393,0.88010764,0.04952507,0.017093642,0.03327036,0.00016235241],"about_ca_topic_score_codex":0.0038794612,"about_ca_topic_score_gemma":0.005149317,"teacher_disagreement_score":0.004063666,"about_ca_system_score_codex":0.0006360839,"about_ca_system_score_gemma":0.0015349875,"threshold_uncertainty_score":0.013594329},"labels":[],"label_agreement":null},{"id":"W2084372305","doi":"10.1086/508599","title":"A Kinematically Selected, Metal‐poor Stellar Halo in the Outskirts of M31","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":146,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Halo; Galactic halo; Andromeda Galaxy; Astronomy; Dark matter halo; Galaxy; Milky Way; Spiral galaxy; Globular cluster; Velocity dispersion; Metallicity; Local Group; Andromeda; Red-giant branch","score_opus":0.005364508760516053,"score_gpt":0.19951041712035625,"score_spread":0.1941459083598402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084372305","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99967396,0.000022221486,0.000032313208,0.000005913262,3.4676168e-7,9.739177e-7,0.00003730531,0.0000035002456,0.00022346884],"genre_scores_gemma":[0.9996463,0.000027742075,0.00005879301,0.000007129253,0.0000018923926,0.0000010623066,0.00013838454,0.0000018865974,0.00011674693],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999323,0.000008096171,0.0000031750417,0.000019016652,0.000012128124,0.000025176329],"domain_scores_gemma":[0.99976593,0.000025429106,0.00009104481,0.000031416148,0.000016428947,0.00006978159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012945011,0.00018441194,0.00021463177,0.0007018101,0.0005743721,0.00039933887,0.0002354391,0.0001865517,0.00077969447],"category_scores_gemma":[0.00038143116,0.00013020428,0.00015619937,0.00054338423,0.00036982243,0.00015943614,0.0006088266,0.00009914214,0.00034383242],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010149376,0.000030138117,0.97354615,0.000013863248,0.00002652698,0.00081694557,0.0006863012,0.00042070443,0.018878967,0.00021169039,0.00021612331,0.0050510922],"study_design_scores_gemma":[0.0000032125702,0.000044624223,0.9977806,0.000003798061,0.000008444225,0.00045037825,0.00022945195,0.00053259457,0.0004966576,0.000108312895,0.00033732754,0.000004559708],"about_ca_topic_score_codex":0.010952576,"about_ca_topic_score_gemma":0.030291773,"teacher_disagreement_score":0.010952576,"about_ca_system_score_codex":0.0003035453,"about_ca_system_score_gemma":0.00021820482,"threshold_uncertainty_score":0.02177763},"labels":[],"label_agreement":null},{"id":"W2084416069","doi":"10.1088/0004-637x/743/2/162","title":"A SEARCH FOR THE TRANSIT OF HD 168443b: IMPROVED ORBITAL PARAMETERS AND PHOTOMETRY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Ephemeris; Photometry (optics); Transit (satellite); Planet; Stars; Exoplanet; Planetary system; Light curve","score_opus":0.026374783669076435,"score_gpt":0.240304196354058,"score_spread":0.21392941268498156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084416069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99464333,0.00013425371,0.002119918,0.00009953026,0.000008366199,0.00004011844,0.0016746119,0.00017575701,0.0011041273],"genre_scores_gemma":[0.97711664,0.000083681676,0.01693152,0.000058338384,0.000029749084,0.000024672268,0.0052271932,0.000034349636,0.0004938983],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998417,0.000019428486,0.000008291432,0.000047819896,0.00004599764,0.00003672134],"domain_scores_gemma":[0.99961144,0.000035636014,0.00010396692,0.000058334615,0.00006865485,0.00012202013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000349067,0.00027338887,0.00026031025,0.0011364607,0.00046930026,0.00036478078,0.00026326015,0.0004203275,0.0013766525],"category_scores_gemma":[0.0004376493,0.00015632511,0.00024053849,0.0009641079,0.00012451247,0.00032247187,0.00038213393,0.0003396889,0.000553006],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007486504,0.00024847116,0.7012952,0.00013757337,0.000072274066,0.00051323284,0.00054632674,0.0017714436,0.18727653,0.00045411274,0.003780895,0.103155255],"study_design_scores_gemma":[0.000036491077,0.00027606546,0.9821186,0.000010852688,0.000037884987,0.00063608296,0.0001313721,0.0033367577,0.0071645854,0.00018602403,0.006045171,0.000020197387],"about_ca_topic_score_codex":0.005913945,"about_ca_topic_score_gemma":0.013346839,"teacher_disagreement_score":0.005913945,"about_ca_system_score_codex":0.00033008854,"about_ca_system_score_gemma":0.00048567334,"threshold_uncertainty_score":0.011759043},"labels":[],"label_agreement":null},{"id":"W2084473899","doi":"10.1088/0004-637x/729/1/20","title":"PULSATIONAL ANALYSIS OF V 588 MON AND V 589 MON OBSERVED WITH THE<i>MOST</i>AND<i>CoRoT</i>SATELLITES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; St. Mary's University; University of British Columbia","funders":"","keywords":"Amplitude; Oscillation (cell signaling); Stars; Spectral line; Rotation (mathematics); Granulation; Noise (video); Residual","score_opus":0.02171467024580868,"score_gpt":0.20763354951008828,"score_spread":0.1859188792642796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084473899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935296,0.00006017871,0.00022152587,0.000046015204,0.000011224494,0.00000604262,0.0008918592,0.000028166432,0.0052053425],"genre_scores_gemma":[0.99785846,0.000030051624,0.00020103251,0.000015830747,0.000011672327,0.000006222938,0.00087393355,0.000015693626,0.0009870888],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999498,0.000003471044,0.0000021262063,0.0000176984,0.000009447404,0.000017460572],"domain_scores_gemma":[0.99983335,0.000029823424,0.00004358111,0.000018849947,0.000031001815,0.000043344102],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011733684,0.00015739693,0.00013987915,0.0008914231,0.0003471442,0.00027907945,0.0001728423,0.00019806896,0.0022862626],"category_scores_gemma":[0.0003026994,0.000118133816,0.00015689078,0.0007289307,0.000119715645,0.00012908119,0.00033412213,0.00022346749,0.00034673407],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011255246,0.000089409485,0.8503231,0.00005724756,0.000084758634,0.0007818596,0.0005910023,0.0021223354,0.10721634,0.001804939,0.002518214,0.033285234],"study_design_scores_gemma":[0.000010056786,0.000027760687,0.9959402,0.0000050328185,0.000014751493,0.0001292032,0.00007022298,0.0010632518,0.0009456103,0.00011164449,0.0016782649,0.000004007614],"about_ca_topic_score_codex":0.005442981,"about_ca_topic_score_gemma":0.011045903,"teacher_disagreement_score":0.005442981,"about_ca_system_score_codex":0.00033018074,"about_ca_system_score_gemma":0.00013671698,"threshold_uncertainty_score":0.010822594},"labels":[],"label_agreement":null},{"id":"W2084492093","doi":"10.1086/382200","title":"Dredge‐up and Envelope Burning in Intermediate‐Mass Giants of Very Low Metallicity","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Metallicity; Envelope (radar); Asymptotic giant branch; Thermal; Convection; Stellar evolution; Stars; Nucleosynthesis; Phase (matter)","score_opus":0.009297354938074216,"score_gpt":0.21916060515921565,"score_spread":0.20986325022114144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084492093","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964425,0.00011000313,0.0016698095,0.00003120559,0.0000025103527,0.0000032417859,0.00007331332,0.000038204733,0.0016291749],"genre_scores_gemma":[0.99890363,0.00004338287,0.00032199488,0.0000061220194,0.0000013340327,0.0000028724264,0.000083969746,0.00000858332,0.00062811316],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999676,0.0000052555083,0.000001474099,0.000007858522,0.0000044959897,0.000013403117],"domain_scores_gemma":[0.9999199,0.000018491733,0.000022299737,0.000007899563,0.0000051978222,0.000026165388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009275779,0.000288963,0.00029470553,0.000376049,0.0003584541,0.00046739265,0.0004806288,0.00040438143,0.0010030961],"category_scores_gemma":[0.00024785905,0.00016856402,0.0006030664,0.00025872077,0.00030033104,0.00026680532,0.000582987,0.00024539663,0.00015884449],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009260708,0.00012632376,0.15376225,0.00016379454,0.00014163181,0.0033679253,0.000524038,0.73173165,0.0800549,0.013267326,0.00047933307,0.015454759],"study_design_scores_gemma":[0.0001069072,0.0004938495,0.19516167,0.000038828603,0.00007402182,0.0011130875,0.00038730598,0.77623796,0.015792854,0.008055502,0.0024731173,0.00006480689],"about_ca_topic_score_codex":0.0052404,"about_ca_topic_score_gemma":0.003561531,"teacher_disagreement_score":0.0052404,"about_ca_system_score_codex":0.0006889074,"about_ca_system_score_gemma":0.00012542933,"threshold_uncertainty_score":0.010419846},"labels":[],"label_agreement":null},{"id":"W2084622335","doi":"10.1088/0004-637x/782/2/88","title":"HOW EMPTY ARE DISK GAPS OPENED BY GIANT PLANETS?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":223,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Giant planet; Surface (topology); Stars; Protoplanet; Viscosity","score_opus":0.007338724394094144,"score_gpt":0.21159736846957058,"score_spread":0.20425864407547645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084622335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935906,0.0005579259,0.0022373125,0.00024152044,0.000012969314,0.0000038219932,0.00007387259,0.00004766021,0.003234401],"genre_scores_gemma":[0.9995278,0.000062639454,0.00025327667,0.000011769403,0.0000049128375,0.0000014585111,0.000021694097,0.0000072264534,0.00010930872],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996929,0.000055855537,0.000013244857,0.00008848951,0.00004658514,0.00010299422],"domain_scores_gemma":[0.99748117,0.0011644303,0.00056068756,0.00022403632,0.00019772569,0.00037193246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036768208,0.00016838778,0.0004145275,0.0005469673,0.00093487,0.0019904787,0.0006187281,0.0007505918,0.0017416751],"category_scores_gemma":[0.0069175833,0.0002739389,0.0001722835,0.000481314,0.0016755834,0.0033859226,0.0009855228,0.00037833033,0.00031144285],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014826962,0.00019244084,0.66660535,0.00049812923,0.00017249052,0.004947109,0.010654536,0.05789423,0.050164983,0.10102513,0.007777568,0.09858535],"study_design_scores_gemma":[0.000105338906,0.00026936838,0.5108009,0.0001690565,0.00013251009,0.0060894853,0.025758225,0.17918746,0.022352759,0.23372689,0.021290729,0.000117321324],"about_ca_topic_score_codex":0.0025214856,"about_ca_topic_score_gemma":0.0018708388,"teacher_disagreement_score":0.0025214856,"about_ca_system_score_codex":0.0005448434,"about_ca_system_score_gemma":0.0002482869,"threshold_uncertainty_score":0.0058264732},"labels":[],"label_agreement":null},{"id":"W2084791911","doi":"10.1088/0004-637x/750/1/1","title":"THE<i>HUBBLE SPACE TELESCOPE</i>CLUSTER SUPERNOVA SURVEY. III. CORRELATED PROPERTIES OF TYPE Ia SUPERNOVAE AND THEIR HOSTS AT 0.9 &lt;<i>z</i>&lt; 1.46","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Supernova; Galaxy; Hubble space telescope; Cluster (spacecraft); Galaxy cluster; Stellar mass; Wide Field Camera 3; Type (biology)","score_opus":0.015154186017959025,"score_gpt":0.21908145890509617,"score_spread":0.20392727288713713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084791911","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94266564,0.0009967319,0.0006522965,0.00015253284,0.00003333055,0.00007951601,0.05128172,0.00013496376,0.0040032347],"genre_scores_gemma":[0.9412171,0.0007766347,0.001105958,0.00006592294,0.000043706998,0.000052847856,0.054011017,0.0000336073,0.0026930736],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997775,0.000034261055,0.000021118576,0.00005109763,0.00006432727,0.000051686937],"domain_scores_gemma":[0.9979705,0.00016212133,0.00082595466,0.0001920749,0.00029156497,0.00055764144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00073509174,0.00040712752,0.0003467182,0.004441608,0.00030046306,0.0005823661,0.00032945408,0.00029219626,0.0020508978],"category_scores_gemma":[0.0010458934,0.00021257276,0.00040300432,0.0023835113,0.00024641675,0.00038861105,0.0005297046,0.00035558926,0.0010252544],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006246187,0.000022801902,0.9923436,0.00002329122,0.000102516955,0.00004763414,0.00005502435,0.00016609418,0.0012536024,0.000107380925,0.0020982863,0.003717248],"study_design_scores_gemma":[0.0000023690036,0.00000931192,0.9990945,0.0000030653032,0.000008421079,0.00002875877,0.000014963999,0.000088650355,0.000106893895,0.000014309297,0.00062741624,0.0000013662681],"about_ca_topic_score_codex":0.029198973,"about_ca_topic_score_gemma":0.06496176,"teacher_disagreement_score":0.029198973,"about_ca_system_score_codex":0.0005698484,"about_ca_system_score_gemma":0.00033891108,"threshold_uncertainty_score":0.058058023},"labels":[],"label_agreement":null},{"id":"W2084836452","doi":"10.1088/0004-637x/781/1/41","title":"<i>CHANDRA</i>AND<i>XMM-NEWTON</i>STUDY OF THE SUPERNOVA REMNANT KES 73 HOSTING THE MAGNETAR 1E 1841-045","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Supernova remnant; Red supergiant; Magnetar; Pulsar; Supernova; Neutron star; Spectral line; Near-Earth supernova","score_opus":0.009929519220923586,"score_gpt":0.2081363603416621,"score_spread":0.19820684112073853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084836452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99734014,0.00053494965,0.000084768835,0.00002204587,0.000003311303,0.000010920868,0.0002102672,0.000015651212,0.0017778574],"genre_scores_gemma":[0.99728346,0.00045211465,0.00086285867,0.000039986455,0.000017220775,0.0000060776447,0.0006671402,0.000008186839,0.0006628976],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998745,0.00001093108,0.000009935575,0.000027115182,0.00003553058,0.000041993047],"domain_scores_gemma":[0.9997223,0.000030265166,0.000095667645,0.000019227642,0.000046837715,0.00008564624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016972085,0.00029444942,0.0002886978,0.0015613091,0.00071316096,0.0004696106,0.0003181618,0.00018888028,0.00079351093],"category_scores_gemma":[0.00025577075,0.00015825262,0.00038057668,0.0009854658,0.0003322161,0.0002731747,0.00041631906,0.0002488303,0.0002525864],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011100435,0.00066276983,0.8332099,0.00028757265,0.00030454795,0.013598889,0.001375118,0.0020046085,0.11256993,0.0009772179,0.0018027879,0.03209668],"study_design_scores_gemma":[0.000008805972,0.00017995451,0.9898336,0.000009791699,0.000039770654,0.0045130868,0.00028716607,0.00041357832,0.0023888918,0.00004399125,0.0022695856,0.000011730367],"about_ca_topic_score_codex":0.011315035,"about_ca_topic_score_gemma":0.016178634,"teacher_disagreement_score":0.011315035,"about_ca_system_score_codex":0.00051677326,"about_ca_system_score_gemma":0.00039993055,"threshold_uncertainty_score":0.02249837},"labels":[],"label_agreement":null},{"id":"W2084921792","doi":"10.1088/0004-637x/745/1/44","title":"THE RISE TIME OF NORMAL AND SUBLUMINOUS TYPE Ia SUPERNOVAE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; University of Toronto; Defence Research and Development Canada; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Supernova; Astrophysics; Physics; Light curve","score_opus":0.011591593702676912,"score_gpt":0.21504725201362107,"score_spread":0.20345565831094417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084921792","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927946,0.00025278883,0.0024839835,0.00001590076,0.000008817099,0.000011631857,0.0013323743,0.00017450159,0.0029254705],"genre_scores_gemma":[0.99320316,0.00015265164,0.0018375071,0.000009358379,0.00001345239,0.000014388988,0.0035237516,0.00007309046,0.0011726057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997627,0.000017816159,0.000019375402,0.00008491455,0.00006758354,0.000047556125],"domain_scores_gemma":[0.998432,0.00030824513,0.0005741251,0.00019357709,0.00021214652,0.00027994317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000507231,0.00024627463,0.000197695,0.0015026224,0.00017850468,0.00058356987,0.00042197213,0.00019319713,0.0016474592],"category_scores_gemma":[0.002428569,0.00017942289,0.00055423554,0.0008679153,0.0001416124,0.00036212374,0.0005316875,0.00033027484,0.00062877056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016568782,0.000027482198,0.958562,0.00005095138,0.00009641286,0.00015170116,0.00018070915,0.0046294667,0.010344277,0.00089945213,0.0004261376,0.02446581],"study_design_scores_gemma":[0.0000024425235,0.000037679518,0.99269205,0.0000038874723,0.00001507338,0.00019719379,0.000024532821,0.003883304,0.0016367611,0.00026701903,0.0012324407,0.000007632671],"about_ca_topic_score_codex":0.0038930415,"about_ca_topic_score_gemma":0.0051030223,"teacher_disagreement_score":0.0038930415,"about_ca_system_score_codex":0.0005341896,"about_ca_system_score_gemma":0.00022500043,"threshold_uncertainty_score":0.0077407956},"labels":[],"label_agreement":null},{"id":"W2084978136","doi":"10.1088/0004-637x/735/1/57","title":"LOCALIZING SAGITTARIUS A* AND M87 ON MICROARCSECOND SCALES WITH MILLIMETER VERY LONG BASELINE INTERFEROMETRY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Very-long-baseline interferometry; Supermassive black hole; Very Long Baseline Array; Stars; Sagittarius A*; Black hole (networking); Milky Way; Quasar; Active galactic nucleus","score_opus":0.018334198559610715,"score_gpt":0.21352653714692105,"score_spread":0.19519233858731033,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2084978136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99054307,0.00022286344,0.0049216035,0.00005901223,0.0000119214965,0.000016128768,0.00037091374,0.00025385286,0.0036005832],"genre_scores_gemma":[0.99168116,0.000052782423,0.0074941367,0.000025246163,0.000013978495,0.000009100726,0.00047382156,0.000016471244,0.00023340838],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990964,0.000012741358,0.0000045409743,0.000025364407,0.00002459249,0.000023200448],"domain_scores_gemma":[0.9997776,0.000020137619,0.00007956081,0.0000413615,0.00003538441,0.000045926183],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019088123,0.00013307505,0.0001360135,0.001117039,0.0001617565,0.00045355974,0.00021954796,0.000198903,0.000590798],"category_scores_gemma":[0.0003535564,0.000107489184,0.00016048277,0.0005005508,0.00015257428,0.00023944795,0.000591632,0.00015625806,0.00033308342],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002255404,0.00006766245,0.70552814,0.000063176085,0.00011979241,0.00023108235,0.00043026695,0.002192191,0.1995799,0.0012415795,0.0016246422,0.08869599],"study_design_scores_gemma":[0.000007394645,0.000058108115,0.9857028,0.000008916107,0.000024789719,0.000108948145,0.00024126777,0.004318152,0.007172925,0.00022746384,0.0021225684,0.0000065334543],"about_ca_topic_score_codex":0.0029402296,"about_ca_topic_score_gemma":0.0062014153,"teacher_disagreement_score":0.0029402296,"about_ca_system_score_codex":0.00018188437,"about_ca_system_score_gemma":0.00011917963,"threshold_uncertainty_score":0.005846262},"labels":[],"label_agreement":null},{"id":"W2085090527","doi":"10.1086/589237","title":"<i>MOST</i> Finds No Coherent Oscillations in the Hot Carbon-rich Wolf-Rayet Star HD 165763 (WR 111)","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Saint Mary's University; University of Toronto; St. Mary's University; University of British Columbia; Herzberg Institute of Astrophysics; Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; Astrophysics; Wolf–Rayet star; Stars; Population; O-type star; Astronomy","score_opus":0.015931381169582228,"score_gpt":0.22458403309971817,"score_spread":0.20865265193013594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085090527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92738044,0.0013208736,0.0015096132,0.0057796864,0.00065018993,0.00004516226,0.004079579,0.00040921196,0.058825243],"genre_scores_gemma":[0.9803612,0.00042022273,0.00095880055,0.0021685122,0.00077463244,0.000016079068,0.005086318,0.00013497265,0.0100792935],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994803,0.00002797843,0.000054937627,0.00016260773,0.00018365415,0.00009057252],"domain_scores_gemma":[0.99596786,0.00077650417,0.0010765231,0.0006946351,0.0009618156,0.0005226865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008170405,0.0003078255,0.00037280525,0.0016508948,0.0011355176,0.0011346466,0.00078304356,0.001526401,0.013899072],"category_scores_gemma":[0.0029286959,0.00019578163,0.00036022687,0.00126005,0.000869273,0.0010261735,0.0010202413,0.00038891923,0.002629946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008744807,0.00012640108,0.80745935,0.00091581536,0.00042120475,0.0038040867,0.0011275711,0.00027930405,0.07968353,0.0012723443,0.044974495,0.05906152],"study_design_scores_gemma":[0.00003877942,0.00022843546,0.94236666,0.00006866168,0.00020683097,0.0034742726,0.0013299247,0.0002334006,0.016123205,0.001236762,0.034649216,0.00004378501],"about_ca_topic_score_codex":0.0021526807,"about_ca_topic_score_gemma":0.00580177,"teacher_disagreement_score":0.013899072,"about_ca_system_score_codex":0.00019175757,"about_ca_system_score_gemma":0.0002163385,"threshold_uncertainty_score":0.046496987},"labels":[],"label_agreement":null},{"id":"W2085130064","doi":"10.1088/0004-637x/702/2/1058","title":"THE DUAL ORIGIN OF STELLAR HALOS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":346,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Ames Research Center; Haverford College; Smithsonian Institution; York University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Galaxy formation and evolution; Halo; Galaxy; Star formation; Accretion (finance); Stars; Population; Milky Way","score_opus":0.008129864156957836,"score_gpt":0.22057980864866175,"score_spread":0.2124499444917039,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085130064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99634546,0.000088673165,0.0017545973,0.000066330715,0.0000047943117,0.0000102222375,0.00008757634,0.000056451834,0.0015859925],"genre_scores_gemma":[0.99887544,0.00003714935,0.00071269186,0.000015831743,0.0000025771124,0.000005756781,0.00009160785,0.000016853095,0.00024195765],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998585,0.00004928828,0.0000060049933,0.00002385529,0.000023388688,0.00003905313],"domain_scores_gemma":[0.99937433,0.00015023816,0.0000940195,0.00007341076,0.0000874358,0.00022057521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005046127,0.00037614055,0.0003673554,0.00046877758,0.00051618984,0.0011698022,0.0007872131,0.0006012233,0.0010618045],"category_scores_gemma":[0.0019489023,0.0003069373,0.0004452628,0.00035733616,0.00070914277,0.0005743781,0.0009413549,0.0003246314,0.00016812723],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003804333,0.00015559442,0.22676566,0.000108108055,0.00026499122,0.0006836117,0.0007882995,0.72635937,0.022560114,0.014506661,0.0008673883,0.0065597063],"study_design_scores_gemma":[0.00016576445,0.000146755,0.047431186,0.00002300039,0.00007531044,0.00018444717,0.00034754816,0.94064754,0.0039989655,0.0048996466,0.0020369813,0.0000429056],"about_ca_topic_score_codex":0.006257677,"about_ca_topic_score_gemma":0.004062703,"teacher_disagreement_score":0.006257677,"about_ca_system_score_codex":0.00077070144,"about_ca_system_score_gemma":0.00041500985,"threshold_uncertainty_score":0.012442529},"labels":[],"label_agreement":null},{"id":"W2085192919","doi":"10.1088/0004-637x/705/2/1395","title":"H I KINEMATICS AND DYNAMICS OF MESSIER 31","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":219,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University; Université de Montréal","funders":"","keywords":"Physics; Galaxy rotation curve; Astrophysics; Dark matter; Halo; Galaxy; Dark matter halo; RADIUS; Mass distribution; Astronomy; Virial theorem; Baryon","score_opus":0.005076874344870079,"score_gpt":0.21074163967202442,"score_spread":0.20566476532715433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085192919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.870136,0.00037324152,0.006802642,0.0010263363,0.00007397491,0.000031068997,0.0005126666,0.0004454235,0.12059863],"genre_scores_gemma":[0.9804494,0.0001049825,0.0010382117,0.00006000709,0.000037686947,0.000009614558,0.00023090458,0.000073550276,0.017995864],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99990773,0.00001245998,0.0000019182637,0.0000293145,0.000014405307,0.000034180335],"domain_scores_gemma":[0.99975413,0.0000293701,0.000045269364,0.000033258348,0.000023515626,0.000114488525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000255851,0.00043507674,0.00040077572,0.0006619094,0.000934195,0.0012594284,0.00039743012,0.0005506869,0.01759293],"category_scores_gemma":[0.0006985791,0.00029359836,0.00035462936,0.00045984212,0.00041553634,0.00094937265,0.0012886451,0.0006577872,0.0023261928],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014085475,0.00019461707,0.16672666,0.00017268247,0.00017548149,0.002926463,0.010577178,0.048726603,0.04553808,0.57787365,0.03389697,0.11178312],"study_design_scores_gemma":[0.00026320652,0.0006456708,0.5850307,0.00013166276,0.00013499963,0.00095093553,0.00584595,0.14568545,0.012422205,0.17286958,0.07576838,0.00025120648],"about_ca_topic_score_codex":0.009604801,"about_ca_topic_score_gemma":0.0067906333,"teacher_disagreement_score":0.01759293,"about_ca_system_score_codex":0.00084140553,"about_ca_system_score_gemma":0.00026801252,"threshold_uncertainty_score":0.058854222},"labels":[],"label_agreement":null},{"id":"W2085194823","doi":"10.1086/497066","title":"Scale Lengths in Dark Matter Halos","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Halo; Instability; Physics; Anisotropy; Isotropy; Dark matter; Length scale; RADIUS; Velocity dispersion; Astrophysics; Power law; Scale (ratio); Classical mechanics; Scale height; Mechanics; Galaxy; Optics; Quantum mechanics; Mathematics; Statistics","score_opus":0.004979285501744264,"score_gpt":0.2059064484098272,"score_spread":0.20092716290808293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085194823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959269,0.000058546062,0.0027986038,0.000065014305,0.0000034131492,0.000004197965,0.00003649602,0.000070352085,0.001036336],"genre_scores_gemma":[0.99922776,0.000027331276,0.0005678396,0.0000055009687,0.0000023052444,0.0000023075318,0.00003351762,0.000014788548,0.00011881861],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999361,0.000015894782,0.0000030053695,0.000014249499,0.000015443644,0.000015315163],"domain_scores_gemma":[0.99918276,0.00024765125,0.00021903387,0.000096878925,0.00006645577,0.00018715335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037313518,0.00022668127,0.00013522673,0.0005374861,0.00035223388,0.0007308083,0.00027073716,0.00020536082,0.000757921],"category_scores_gemma":[0.0028930425,0.00019449818,0.00029492562,0.00027042322,0.00051458564,0.0006170589,0.00058113155,0.00028556233,0.000074435535],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005194298,0.00011632295,0.16341878,0.00012470353,0.00019392994,0.0009619002,0.0012547063,0.6770445,0.076591976,0.06614853,0.0011160601,0.012509136],"study_design_scores_gemma":[0.00012420025,0.00014926234,0.070365496,0.000020396792,0.00004080827,0.00016743314,0.0002223788,0.8808765,0.0127444705,0.034045115,0.0011889993,0.000054972006],"about_ca_topic_score_codex":0.002672119,"about_ca_topic_score_gemma":0.00172724,"teacher_disagreement_score":0.002672119,"about_ca_system_score_codex":0.00063862215,"about_ca_system_score_gemma":0.0002041864,"threshold_uncertainty_score":0.005313158},"labels":[],"label_agreement":null},{"id":"W2085207267","doi":"10.1088/0004-637x/775/1/21","title":"THE FADING OF TWO TRANSIENT ULTRALUMINOUS X-RAY SOURCES TO BELOW THE STELLAR MASS EDDINGTON LIMIT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; X-ray transient; Luminosity; Black hole (networking); Galaxy; Eddington luminosity; Astronomy; Neutron star","score_opus":0.011441933618377456,"score_gpt":0.22495995175691932,"score_spread":0.21351801813854188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085207267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983777,0.00012532626,0.00052242965,0.000029145132,0.000004881489,0.0000037765608,0.00011848565,0.00003864691,0.000779682],"genre_scores_gemma":[0.9984665,0.00005058162,0.00065592333,0.000026980619,0.000010178112,0.0000042287697,0.00035253182,0.0000074955137,0.00042549294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985254,0.000008131652,0.000009084483,0.00004701173,0.00003938217,0.000043869048],"domain_scores_gemma":[0.9987865,0.00015457382,0.00047132937,0.00017802574,0.00014967956,0.00025983693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030015153,0.00023852603,0.00022113178,0.00078853784,0.00043731774,0.00077181746,0.00046435025,0.00036713987,0.00095821236],"category_scores_gemma":[0.0009063644,0.00017979486,0.00015946898,0.0005442986,0.00034207472,0.0004152356,0.00070793275,0.00042721603,0.00024019336],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047940935,0.000097745615,0.89379895,0.00007476263,0.0000534176,0.0014308597,0.0009175712,0.0004248784,0.072727956,0.00059334695,0.0004693772,0.028931713],"study_design_scores_gemma":[0.000006133454,0.000100168014,0.9923281,0.000009135804,0.00001558633,0.0008794863,0.00011254,0.0005787146,0.004550068,0.000100074045,0.0013108589,0.000009235247],"about_ca_topic_score_codex":0.002567221,"about_ca_topic_score_gemma":0.005234698,"teacher_disagreement_score":0.002567221,"about_ca_system_score_codex":0.00033346025,"about_ca_system_score_gemma":0.00014299415,"threshold_uncertainty_score":0.0051046014},"labels":[],"label_agreement":null},{"id":"W2085292733","doi":"10.1086/524350","title":"The Environment of M85 Optical Transient 2006‐1: Constraints on the Progenitor Age and Mass","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Galaxy; Astrophysics; Astronomy; Star cluster; Stars; Stellar evolution","score_opus":0.008686060474814673,"score_gpt":0.18808071995070846,"score_spread":0.17939465947589378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085292733","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975706,0.00018754906,0.00021180022,0.000034310127,0.0000026398407,0.0000028105649,0.00013806453,0.000018225466,0.0018340203],"genre_scores_gemma":[0.99904674,0.000088966255,0.0003040234,0.000027843189,0.000005348681,0.000002011061,0.0003033156,0.000006420364,0.0002152036],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995494,0.0000023359655,0.0000024479564,0.000014702539,0.000008983077,0.000016605925],"domain_scores_gemma":[0.9998301,0.000012215028,0.00008091443,0.0000140407865,0.000014185784,0.000048502123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014815216,0.00016601314,0.00019112909,0.00040359964,0.00050953665,0.00072099094,0.0003364538,0.00037940987,0.0010343938],"category_scores_gemma":[0.00027128728,0.00015193115,0.00014159364,0.00026923904,0.0001634301,0.00034016656,0.00046580614,0.00024153567,0.0004385018],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044196978,0.00008562485,0.8744784,0.00007410977,0.000032993004,0.0007320461,0.0007100703,0.001315295,0.10248289,0.0016047229,0.0007636997,0.0172782],"study_design_scores_gemma":[0.00000780057,0.000069870366,0.9897265,0.000015547039,0.000021397556,0.00040007726,0.0002586973,0.0027789862,0.0039737914,0.00019241848,0.002546968,0.0000079495985],"about_ca_topic_score_codex":0.003923755,"about_ca_topic_score_gemma":0.0069114957,"teacher_disagreement_score":0.003923755,"about_ca_system_score_codex":0.00053494266,"about_ca_system_score_gemma":0.00019746895,"threshold_uncertainty_score":0.007801831},"labels":[],"label_agreement":null},{"id":"W2085411824","doi":"10.1088/0004-637x/741/1/55","title":"ORBITAL MOTION OF HR 8799 b, c, d USING<i>HUBBLE SPACE TELESCOPE</i>DATA FROM 1998: CONSTRAINTS ON INCLINATION, ECCENTRICITY, AND STABILITY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrometry; Physics; Planet; Exoplanet; Astronomy; Coronagraph; Planetary system; Proper motion; Orbital eccentricity; Mean motion; Astrophysics; Orbital motion; Orbital inclination; Giant planet; Stars; Binary number; Classical mechanics; Angular momentum","score_opus":0.047885224128980754,"score_gpt":0.25441498036094834,"score_spread":0.2065297562319676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085411824","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99503976,0.00007973475,0.00027620883,0.000017915332,0.0000027888905,0.000009235084,0.002979992,0.000042489974,0.0015518726],"genre_scores_gemma":[0.9884291,0.000055382312,0.0012923424,0.000009220286,0.000007508646,0.000009075468,0.009896637,0.000014703556,0.00028599394],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986875,0.0000130330045,0.000009659294,0.000040602663,0.0000378847,0.000030039655],"domain_scores_gemma":[0.99964726,0.000047027457,0.00010074431,0.00007851649,0.000066334585,0.000060165155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023158682,0.00018512864,0.00019883568,0.0018340749,0.00040938478,0.000503715,0.00022886405,0.00020985129,0.0007937086],"category_scores_gemma":[0.00050555705,0.000113136484,0.00022357277,0.0014534032,0.00015749091,0.00015225788,0.0002784663,0.00023703833,0.00045656503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059671025,0.00022458614,0.8832747,0.00007931996,0.00011704287,0.0004907918,0.00051621255,0.005638436,0.04745556,0.00044864186,0.0046011363,0.056556802],"study_design_scores_gemma":[0.000009674514,0.000016013402,0.9933989,0.000007179033,0.000016364642,0.000069027934,0.000043979428,0.0033368259,0.0017666105,0.00002758729,0.0013031494,0.0000047757358],"about_ca_topic_score_codex":0.027482478,"about_ca_topic_score_gemma":0.039306432,"teacher_disagreement_score":0.027482478,"about_ca_system_score_codex":0.0006000392,"about_ca_system_score_gemma":0.00029881444,"threshold_uncertainty_score":0.054645002},"labels":[],"label_agreement":null},{"id":"W2085480081","doi":"10.1088/0004-637x/771/2/109","title":"SEARCH FOR RAYLEIGH SCATTERING IN THE ATMOSPHERE OF GJ1214b","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Atmosphere (unit); Planet; Physics; Rayleigh scattering; Exoplanet; Scale height; Telescope; Transit (satellite); Wavelength; Spectrograph; RADIUS; Astronomy; Astrophysics; Optics; Meteorology; Spectral line","score_opus":0.015259055968534076,"score_gpt":0.24064875790299586,"score_spread":0.22538970193446178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085480081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877936,0.000051078074,0.00012387193,0.000065541404,0.0000029048824,0.0000053032945,0.00015752898,0.000048375707,0.000766207],"genre_scores_gemma":[0.99881506,0.000023335355,0.00023276711,0.000028867658,0.000007676492,0.0000062006557,0.0006434314,0.000009991401,0.00023275932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998759,0.00001255939,0.0000050295343,0.000035254765,0.000034061453,0.00003722896],"domain_scores_gemma":[0.999666,0.000037272865,0.00009229135,0.000026946624,0.00004245092,0.000135181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021578064,0.00033803147,0.00025840744,0.0015006198,0.0007717998,0.00048851606,0.00034470792,0.0005514475,0.0011106075],"category_scores_gemma":[0.00044587418,0.00034940545,0.00027090163,0.00050638634,0.0002811859,0.00030332254,0.00061143324,0.00035125285,0.000404639],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037688584,0.00022993289,0.75535935,0.000046812256,0.00014410655,0.00074792653,0.0007873043,0.0014995631,0.22815606,0.0006159388,0.001619153,0.010417026],"study_design_scores_gemma":[0.000022250537,0.00007300013,0.99301964,0.0000035375992,0.000019970128,0.00015588665,0.00015862231,0.0027168153,0.002889807,0.00006292566,0.0008677959,0.000009601494],"about_ca_topic_score_codex":0.010535074,"about_ca_topic_score_gemma":0.0078030713,"teacher_disagreement_score":0.010535074,"about_ca_system_score_codex":0.00054205063,"about_ca_system_score_gemma":0.00024896485,"threshold_uncertainty_score":0.020947456},"labels":[],"label_agreement":null},{"id":"W2085543184","doi":"10.1088/0004-637x/707/2/1740","title":"BLAST: A FAR-INFRARED MEASUREMENT OF THE HISTORY OF STAR FORMATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Redshift; Luminosity; Star formation; Galaxy; Infrared; Astronomy; Far infrared; Cosmic infrared background; Surface brightness; Luminous infrared galaxy; Extragalactic background light; Cosmic microwave background","score_opus":0.012103119483176493,"score_gpt":0.19109125327783247,"score_spread":0.17898813379465597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085543184","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97526574,0.0004585821,0.004898531,0.000076087956,0.000022000208,0.00007751433,0.009188175,0.0005397211,0.009473582],"genre_scores_gemma":[0.98118883,0.00026438915,0.008890987,0.0000628579,0.00006521027,0.00004384976,0.00820877,0.000035169982,0.0012399253],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973124,0.000035381854,0.000012836304,0.00007063214,0.000112806665,0.000037002224],"domain_scores_gemma":[0.999,0.000109238805,0.00049922185,0.00012600726,0.00009249614,0.00017301216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005295688,0.00031603684,0.0002918744,0.0014991823,0.00022615948,0.00041233265,0.00038080823,0.00026639152,0.0015270298],"category_scores_gemma":[0.0007533697,0.0002308265,0.00023326949,0.0015722734,0.0002794927,0.00040674873,0.00053139316,0.00028819428,0.00069488765],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036548957,0.00012266384,0.9262881,0.00013017423,0.00014253565,0.000118105585,0.0002967521,0.0014594035,0.039641626,0.0010414207,0.0021008868,0.028292863],"study_design_scores_gemma":[0.000009467018,0.00006810333,0.9949763,0.0000042903534,0.000016995658,0.00011889683,0.000022603539,0.0008167028,0.0023336282,0.00016624745,0.0014606008,0.000006132943],"about_ca_topic_score_codex":0.0025081434,"about_ca_topic_score_gemma":0.0063098753,"teacher_disagreement_score":0.0025081434,"about_ca_system_score_codex":0.00035770462,"about_ca_system_score_gemma":0.00016787238,"threshold_uncertainty_score":0.0051084757},"labels":[],"label_agreement":null},{"id":"W2085597769","doi":"10.1086/524649","title":"A Jet Associated with the Classical T Tauri Star RY Tauri","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Physics; T Tauri star; Astrophysics; Position angle; Proper motion; Astronomy; Hubble space telescope; Herbig–Haro object; Jet (fluid); Star formation; Stars; Galaxy","score_opus":0.010619582959508751,"score_gpt":0.19512551355561644,"score_spread":0.1845059305961077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085597769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970613,0.0005314741,0.0005138161,0.000031070445,0.000015906595,0.0000057420525,0.000294935,0.00003709882,0.0015086838],"genre_scores_gemma":[0.9969549,0.00031849867,0.0013844072,0.000026550126,0.000039537317,0.000004348062,0.00082715706,0.000008600687,0.00043587072],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999387,0.000004488218,0.0000043547625,0.000018421551,0.000014214248,0.00001972074],"domain_scores_gemma":[0.9996581,0.000049252183,0.00013459567,0.00004811016,0.000036728215,0.00007331643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012004487,0.00016042063,0.00017344025,0.00062946876,0.00029940077,0.0005722462,0.00022623347,0.0002755044,0.0010615289],"category_scores_gemma":[0.00028287937,0.00013395605,0.00017192184,0.00071172667,0.00031656696,0.00018942912,0.0003098947,0.00025174374,0.00023559945],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016190775,0.00013559582,0.21959068,0.0004200214,0.00016284197,0.01738621,0.0009778163,0.00085040304,0.72156304,0.0028543985,0.0018659467,0.03257405],"study_design_scores_gemma":[0.00006152177,0.00030220166,0.9613733,0.000027585178,0.000059686987,0.013177446,0.00024034962,0.0011271155,0.018808288,0.00045684451,0.004345232,0.00002044938],"about_ca_topic_score_codex":0.0013319738,"about_ca_topic_score_gemma":0.0016341584,"teacher_disagreement_score":0.0013319738,"about_ca_system_score_codex":0.00023916225,"about_ca_system_score_gemma":0.000074238174,"threshold_uncertainty_score":0.0035511851},"labels":[],"label_agreement":null},{"id":"W2085609620","doi":"10.1086/505214","title":"Production of the Extended Scattered Disk by Rogue Planets","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Planet; Exoplanet; Astrobiology; Astronomy; Planetary system; Astrophysics","score_opus":0.00412491771806505,"score_gpt":0.18524152275786648,"score_spread":0.18111660503980143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085609620","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971765,0.00044737995,0.0010994195,0.000015191665,0.000004101137,0.0000028219465,0.00002563497,0.000011297499,0.0012176046],"genre_scores_gemma":[0.9990984,0.00012890718,0.00029182938,0.0000057296147,0.0000039798288,0.0000019242716,0.0000708056,0.0000019157903,0.00039650846],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998549,0.000028001945,0.000006754908,0.000047123212,0.000025756433,0.000037355534],"domain_scores_gemma":[0.9987029,0.00035184383,0.00034718146,0.00039955802,0.000070056725,0.00012847956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003216364,0.00024000884,0.0001892576,0.0003556727,0.0003329834,0.000593735,0.000310878,0.00025081943,0.0015937225],"category_scores_gemma":[0.0010407675,0.00014752007,0.00023781412,0.00015738973,0.00036780268,0.00046789012,0.0007531576,0.00022374318,0.0005571672],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094842527,0.00023257128,0.6099049,0.00014673446,0.00020282267,0.005750115,0.00063502125,0.0044877455,0.33635563,0.0056436243,0.0004650363,0.035227455],"study_design_scores_gemma":[0.00010589142,0.0020736915,0.6485966,0.000047118,0.00022182493,0.042075437,0.0009166311,0.027352419,0.25555617,0.0055121626,0.01747951,0.00006257605],"about_ca_topic_score_codex":0.00022708104,"about_ca_topic_score_gemma":0.0002208383,"teacher_disagreement_score":0.0015937225,"about_ca_system_score_codex":0.00013905171,"about_ca_system_score_gemma":0.00006170277,"threshold_uncertainty_score":0.0053315163},"labels":[],"label_agreement":null},{"id":"W2085636267","doi":"10.1088/0004-637x/743/2/111","title":"THE THERMAL STRUCTURE OF GRAVITATIONALLY DARKENED CLASSICAL Be STAR DISKS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Rotation (mathematics); Stellar rotation; Gravitational energy; Thin disk; Gravitation; Rotation period; Stars; Gravitational field; Astronomy; Gravitational wave; Geometry","score_opus":0.015480961309362253,"score_gpt":0.22512821557910997,"score_spread":0.20964725426974773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085636267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9909462,0.00024896322,0.0063164104,0.000060047536,0.0000065112235,0.000012126621,0.00010272349,0.000053904856,0.0022531298],"genre_scores_gemma":[0.99797684,0.00014511864,0.0012951206,0.0000115883795,0.000005122987,0.0000077672585,0.00012073134,0.000025786137,0.00041195127],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998447,0.000055335793,0.000008906487,0.000034682955,0.000026524387,0.000029733199],"domain_scores_gemma":[0.9991886,0.0002667645,0.00017896762,0.00012786544,0.00012373114,0.00011399451],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039826034,0.00056615967,0.00043317376,0.00053182716,0.0005575725,0.0010403179,0.001054247,0.00045781644,0.00082201697],"category_scores_gemma":[0.0019301405,0.0003841454,0.0004461567,0.00037152195,0.00094449305,0.0009902564,0.0005961574,0.00037785398,0.000104144885],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019621468,0.00004975165,0.01595774,0.000048192953,0.000062568986,0.000144315,0.00009582093,0.9685259,0.007831372,0.00536873,0.000120405726,0.0015989235],"study_design_scores_gemma":[0.000026985252,0.000057189434,0.006220851,0.0000070045935,0.000014836957,0.000046010664,0.000031890235,0.988112,0.0019041523,0.003376665,0.00018739644,0.0000150991045],"about_ca_topic_score_codex":0.005552689,"about_ca_topic_score_gemma":0.0030714062,"teacher_disagreement_score":0.005552689,"about_ca_system_score_codex":0.0011766736,"about_ca_system_score_gemma":0.00028355038,"threshold_uncertainty_score":0.011040747},"labels":[],"label_agreement":null},{"id":"W2085700480","doi":"10.1088/0004-637x/759/2/102","title":"VERITAS OBSERVATIONS OF SIX BRIGHT, HARD-SPECTRUM<i>FERMI</i>-LAT BLAZARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Office of Science; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; National Science Foundation; Agenzia Spaziale Italiana; Max-Planck-Gesellschaft; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Alfred P. Sloan Foundation; Jet Propulsion Laboratory; Ministry of Education, Culture, Sports, Science and Technology; Japan Aerospace Exploration Agency; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; Science Foundation Ireland","keywords":"Blazar; Physics; Astrophysics; Fermi Gamma-ray Space Telescope; Extragalactic background light; Redshift; Astronomy; Telescope; Synchrotron; Active galactic nucleus; Galaxy; Sky; Spectral energy distribution; Gamma ray; Optics","score_opus":0.019895133988008584,"score_gpt":0.2260300740260553,"score_spread":0.20613494003804672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085700480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950329,0.00015722436,0.00041941533,0.0000486248,0.000008834913,0.000011186061,0.0015172025,0.000118403885,0.0026861464],"genre_scores_gemma":[0.99279904,0.000098416574,0.0019385954,0.00004228854,0.00002131117,0.000009799357,0.0040013287,0.000031018517,0.0010581409],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997929,0.000013389726,0.000009859415,0.000055952827,0.000058587473,0.00006924919],"domain_scores_gemma":[0.999464,0.00006420599,0.00020182368,0.0000744495,0.00006441648,0.00013107769],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035428247,0.00033597942,0.00024301265,0.0011913327,0.0006401876,0.0006069017,0.00034871363,0.00030777036,0.0018546617],"category_scores_gemma":[0.0005263742,0.00027900125,0.00027205472,0.00044681318,0.00025008587,0.00028248024,0.0006011935,0.00035832578,0.00042563945],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014801292,0.00021946638,0.83128005,0.00012073674,0.00024972466,0.0012384215,0.0022329385,0.001740481,0.0972296,0.0017680025,0.005723897,0.056716613],"study_design_scores_gemma":[0.00007870727,0.00024169465,0.9847676,0.000027340266,0.00007433131,0.00064395263,0.00019941056,0.0012192694,0.0053662467,0.0002272593,0.0071301493,0.000024008894],"about_ca_topic_score_codex":0.014264277,"about_ca_topic_score_gemma":0.027690627,"teacher_disagreement_score":0.014264277,"about_ca_system_score_codex":0.00075538945,"about_ca_system_score_gemma":0.00024328804,"threshold_uncertainty_score":0.028362513},"labels":[],"label_agreement":null},{"id":"W2085892310","doi":"10.1086/342175","title":"The Broadband Afterglow of GRB 980329","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Afterglow; Gamma-ray burst; Physics; Ejecta; Astrophysics; Redshift; Galaxy; Astronomy; Broadband; Light curve; Collimated light; Supernova; Optics","score_opus":0.010349187112222566,"score_gpt":0.2115948574340545,"score_spread":0.20124567032183194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085892310","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961481,0.0002253627,0.00063448976,0.000030503597,0.000014653734,0.00000838067,0.0012289692,0.000107060194,0.0016025472],"genre_scores_gemma":[0.99597293,0.0001543645,0.00041855426,0.00002819179,0.000013653124,0.000008686559,0.0030633537,0.000019526353,0.00032082456],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999113,0.0000091836355,0.000005475986,0.000026749862,0.000015351867,0.000031929165],"domain_scores_gemma":[0.9995103,0.0000499257,0.00021784699,0.000046138157,0.000047357273,0.0001284926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016217255,0.00037445955,0.00031068662,0.000789023,0.00028386494,0.0004425689,0.0003000248,0.0004337688,0.00095116446],"category_scores_gemma":[0.00036298297,0.00014019641,0.000375066,0.0008079492,0.00013599223,0.00024778483,0.00044130845,0.0003866422,0.000578105],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010550093,0.00035415025,0.8865253,0.00017542538,0.00019672657,0.0021459353,0.0003528905,0.006377246,0.063151486,0.0014456717,0.0036137707,0.034606334],"study_design_scores_gemma":[0.000015989799,0.00010433969,0.9916187,0.000022968134,0.000033190234,0.0008088551,0.000055660308,0.0033790753,0.0012994175,0.0002661929,0.0023798572,0.000015903206],"about_ca_topic_score_codex":0.0026746565,"about_ca_topic_score_gemma":0.004100525,"teacher_disagreement_score":0.0026746565,"about_ca_system_score_codex":0.00022408922,"about_ca_system_score_gemma":0.000088169894,"threshold_uncertainty_score":0.005318165},"labels":[],"label_agreement":null},{"id":"W2085911439","doi":"10.1088/0004-637x/758/2/137","title":"H II REGION VARIABILITY AND PRE-MAIN-SEQUENCE EVOLUTION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Protostar; Radiative transfer; RADIUS; Stars; Stellar evolution; Flux (metallurgy); Computational astrophysics; Numerical models","score_opus":0.014673181631869038,"score_gpt":0.24712537429344253,"score_spread":0.2324521926615735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2085911439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998755,0.000056657093,0.00033771328,0.000023233251,0.000002696445,0.000003207548,0.00007408389,0.000018074756,0.0007292834],"genre_scores_gemma":[0.9996406,0.00003210617,0.00008335716,0.0000070663423,0.0000017221364,0.0000017930778,0.000092901486,0.0000053220856,0.00013523431],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999946,0.000008503454,0.000002991337,0.000017571692,0.0000072308417,0.000017683486],"domain_scores_gemma":[0.99971455,0.000072771356,0.00007751326,0.000024852745,0.000018411274,0.00009199635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021818609,0.00028354174,0.0002562433,0.00021785371,0.00032447177,0.0007315863,0.00043644963,0.0005922099,0.001594174],"category_scores_gemma":[0.0008803307,0.00020684351,0.00046462278,0.00019978665,0.00029366472,0.00051483023,0.00036025932,0.0003716537,0.00025885671],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004491686,0.000219014,0.55732244,0.000076192184,0.00023096998,0.000795245,0.00036123133,0.38909397,0.039206218,0.005977004,0.00049664953,0.0057720197],"study_design_scores_gemma":[0.00010572866,0.0003716804,0.491654,0.000014534413,0.000070324495,0.00032668049,0.00023304757,0.49923122,0.003691435,0.0034494977,0.0008178517,0.000034006378],"about_ca_topic_score_codex":0.0056504915,"about_ca_topic_score_gemma":0.0049929447,"teacher_disagreement_score":0.0056504915,"about_ca_system_score_codex":0.00077228947,"about_ca_system_score_gemma":0.00030175518,"threshold_uncertainty_score":0.0112351775},"labels":[],"label_agreement":null},{"id":"W2086018342","doi":"10.1088/0004-637x/715/2/1419","title":"THE ADVANCED CAMERA FOR SURVEYS FORNAX CLUSTER SURVEY. VII. HALF-LIGHT RADII OF GLOBULAR CLUSTERS IN EARLY-TYPE GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Virgo Cluster; Effective radius; Galaxy; RADIUS; Cluster (spacecraft); Galaxy cluster; Astronomy","score_opus":0.007210265278538103,"score_gpt":0.22619937662037995,"score_spread":0.21898911134184185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086018342","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22145684,0.0016354388,0.0049084104,0.0012570613,0.00031539422,0.00061867904,0.6869183,0.0069115595,0.075978346],"genre_scores_gemma":[0.2983643,0.0012632405,0.045127615,0.00092945277,0.000442,0.0010070418,0.6002914,0.0012256246,0.05134931],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9994141,0.00006404416,0.000030283521,0.00015002192,0.0002631912,0.00007838029],"domain_scores_gemma":[0.99843615,0.0000744505,0.00044927542,0.00028099472,0.00047746644,0.00028153922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077499764,0.00062258675,0.00043983306,0.0030541862,0.00048273493,0.0008008838,0.00068055757,0.00047852893,0.01126966],"category_scores_gemma":[0.0013829384,0.00025836952,0.0003506595,0.0020273959,0.00017093177,0.000834351,0.0010291081,0.0006570181,0.008808631],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002558476,0.00015894623,0.36141112,0.00031143674,0.0002164178,0.00015811925,0.0005204653,0.0005537424,0.005785764,0.0029587634,0.5387788,0.08889071],"study_design_scores_gemma":[0.00007128598,0.000041873143,0.7829712,0.000048197395,0.00004022479,0.00012217903,0.0002136456,0.0012266911,0.0011897794,0.0006017638,0.2134464,0.000026690666],"about_ca_topic_score_codex":0.030132405,"about_ca_topic_score_gemma":0.04344657,"teacher_disagreement_score":0.030132405,"about_ca_system_score_codex":0.0007798512,"about_ca_system_score_gemma":0.0005956656,"threshold_uncertainty_score":0.059914052},"labels":[],"label_agreement":null},{"id":"W2086090890","doi":"10.1086/378497","title":"Polarization of Prompt Gamma‐Ray Burst Emission: Evidence for Electromagnetically Dominated Outflow","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":265,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Gamma-ray burst; Magnetic field; Polarization (electrochemistry); Astrophysics; Lorentz factor; Outflow; Stokes parameters; Linear polarization; Plasma; Computational physics; Scattering; Lorentz transformation; Optics; Classical mechanics; Nuclear physics; Laser; Quantum mechanics","score_opus":0.015232316654952765,"score_gpt":0.2584656820161729,"score_spread":0.24323336536122017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086090890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979978,0.000110584,0.0008050438,0.000016589998,0.0000034256982,0.0000021992737,0.00007690394,0.000034263077,0.0009532123],"genre_scores_gemma":[0.999403,0.000076079734,0.00028798988,0.0000073678025,0.0000068223803,0.0000020108534,0.00013421208,0.0000061717597,0.00007638836],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995327,0.000008794103,0.0000033122626,0.00001291867,0.000009534791,0.00001213459],"domain_scores_gemma":[0.9997694,0.00006302483,0.000071701135,0.000035721205,0.000026969154,0.000033144734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015531479,0.00017065703,0.000107700434,0.00046405,0.00015204259,0.0005340839,0.0001432025,0.00023144156,0.00064691843],"category_scores_gemma":[0.000441442,0.0001670545,0.0001235494,0.000272776,0.00031195785,0.00017781294,0.0002691061,0.00017213325,0.00020212673],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009851445,0.00014068001,0.52648664,0.0001057492,0.000062805746,0.0011990962,0.00038529874,0.0032945792,0.44040406,0.0020616665,0.0006168935,0.024257446],"study_design_scores_gemma":[0.000102029764,0.00019959186,0.914228,0.000020653226,0.0000655463,0.0035999846,0.0001959856,0.016720125,0.060817115,0.0024864518,0.0015406938,0.000023876139],"about_ca_topic_score_codex":0.00027725645,"about_ca_topic_score_gemma":0.00022411316,"teacher_disagreement_score":0.00064691843,"about_ca_system_score_codex":0.00011511258,"about_ca_system_score_gemma":0.00006087153,"threshold_uncertainty_score":0.002164185},"labels":[],"label_agreement":null},{"id":"W2086190933","doi":"10.1088/0004-637x/691/2/1595","title":"THE ARECIBO LEGACY FAST ALFA SURVEY. VII. A NEUTRAL HYDROGEN CLOUD COMPLEX IN THE VIRGO CLUSTER","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Virgo Cluster; Physics; Astrophysics; Galaxy; Astronomy; Halo; Galaxy cluster; Cluster (spacecraft); Intracluster medium; Dark matter","score_opus":0.014642666552404027,"score_gpt":0.23590741900193715,"score_spread":0.22126475244953311,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086190933","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8081427,0.0026300568,0.0008713094,0.0006423395,0.0001289856,0.0002720156,0.13960676,0.00048898783,0.047216825],"genre_scores_gemma":[0.78953767,0.0020893835,0.004844612,0.0004095063,0.0001981933,0.00015521797,0.18782687,0.00019800363,0.014740488],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997948,0.000014618708,0.0000075904527,0.00004229474,0.00006913458,0.00007157527],"domain_scores_gemma":[0.9996375,0.000015080395,0.00009593671,0.000053948144,0.00006579432,0.00013173837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029173723,0.000429796,0.00038277055,0.0030457883,0.0007368129,0.000737934,0.00052684377,0.00045270578,0.0035438638],"category_scores_gemma":[0.00028694436,0.00017311411,0.00019712391,0.002470445,0.00014307925,0.00027137678,0.0007142799,0.00030120305,0.0024428905],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081094005,0.0003189483,0.7632841,0.000373516,0.00023395657,0.001211249,0.001560799,0.0007096032,0.023228472,0.0018861224,0.13862993,0.06775238],"study_design_scores_gemma":[0.0000343961,0.000041971398,0.936938,0.000029948844,0.000026258269,0.00029037782,0.00030878445,0.0003736221,0.0006637234,0.000099571815,0.06118026,0.000013062361],"about_ca_topic_score_codex":0.0887037,"about_ca_topic_score_gemma":0.13878421,"teacher_disagreement_score":0.0887037,"about_ca_system_score_codex":0.00092893164,"about_ca_system_score_gemma":0.0004363633,"threshold_uncertainty_score":0.17637473},"labels":[],"label_agreement":null},{"id":"W2086211578","doi":"10.1088/0004-637x/700/1/10","title":"DISPERSAL OF PROTOPLANETARY DISKS BY CENTRAL WIND STRIPPING","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Outflow; Accretion (finance); Photoevaporation; Entrainment (biomusicology); Protoplanetary disk; Turbulence; Wind speed; Scale height","score_opus":0.006966031131939469,"score_gpt":0.22383984798826798,"score_spread":0.2168738168563285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086211578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9127948,0.002150832,0.058985762,0.0018581849,0.00016110808,0.00013942103,0.0005113719,0.00034127795,0.02305717],"genre_scores_gemma":[0.9845575,0.00068008096,0.003163094,0.000119537384,0.000066114735,0.000065219836,0.0001397639,0.000033123848,0.011175537],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999198,0.000014544824,0.0000033784092,0.000026110916,0.000013004467,0.00002325662],"domain_scores_gemma":[0.999759,0.000039000603,0.000069474714,0.000034086264,0.000019623438,0.00007873253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019885882,0.0006863631,0.0005681785,0.00030227433,0.00079491857,0.0012702177,0.0016976222,0.0017836043,0.0028986807],"category_scores_gemma":[0.0008089688,0.00035190376,0.00087215647,0.00022049806,0.0008401073,0.0018608121,0.001124982,0.00056600355,0.00094272563],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004420802,0.00021866469,0.018422998,0.00020198546,0.00011764529,0.003204939,0.0005900882,0.89035183,0.012719112,0.05858684,0.0036358058,0.011508115],"study_design_scores_gemma":[0.00035747394,0.00023431644,0.0047313753,0.000034897217,0.00005370397,0.0011822246,0.0002041327,0.96689945,0.00087082415,0.021618862,0.0037625073,0.000050317118],"about_ca_topic_score_codex":0.009538518,"about_ca_topic_score_gemma":0.0034429368,"teacher_disagreement_score":0.009538518,"about_ca_system_score_codex":0.0010846376,"about_ca_system_score_gemma":0.00047687895,"threshold_uncertainty_score":0.01896602},"labels":[],"label_agreement":null},{"id":"W2086324543","doi":"10.1086/382020","title":"Using Narrowband Photometry to Classify Stars and Brown Dwarfs","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Brown dwarf; Stellar classification; Astrophysics; Physics; Stars; Photometry (optics); Astronomy","score_opus":0.02239411988015272,"score_gpt":0.25976784688692367,"score_spread":0.23737372700677095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086324543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.85594195,0.00024779732,0.1353332,0.000086915315,0.000021449194,0.00008485069,0.00065348536,0.0011970784,0.0064332983],"genre_scores_gemma":[0.9444547,0.000084825544,0.05357708,0.000041105497,0.0000074758227,0.000034493823,0.00066645513,0.000052480853,0.0010814411],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963,0.0000615091,0.00002145948,0.00012798731,0.0001155675,0.00004352473],"domain_scores_gemma":[0.9988662,0.0002886059,0.00022283835,0.00018633674,0.00028559985,0.00015048016],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007746115,0.0003723451,0.0002872353,0.0015477865,0.0004135317,0.0008613532,0.00038525218,0.00046086413,0.00087195827],"category_scores_gemma":[0.0019733505,0.00019543883,0.00046986406,0.00059016765,0.00039741574,0.000667276,0.00040887893,0.0002525698,0.0008890819],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027586063,0.00012235848,0.7953384,0.000060159764,0.000108125656,0.00009872087,0.00031039308,0.046494227,0.037620418,0.0023237052,0.0010102689,0.11623731],"study_design_scores_gemma":[0.00006484013,0.00039905557,0.5509434,0.00005914457,0.000119520904,0.0004353844,0.00039990703,0.39454576,0.033565316,0.011419763,0.007929136,0.00011882241],"about_ca_topic_score_codex":0.013166238,"about_ca_topic_score_gemma":0.018153297,"teacher_disagreement_score":0.013166238,"about_ca_system_score_codex":0.00084389787,"about_ca_system_score_gemma":0.000482198,"threshold_uncertainty_score":0.026179254},"labels":[],"label_agreement":null},{"id":"W2086328762","doi":"10.1088/0004-637x/698/2/l116","title":"STAR FORMATION AND DUST OBSCURATION AT <i>z</i> ≈ 2: GALAXIES AT THE DAWN OF DOWNSIZING","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":368,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Astrophysics; Physics; Star formation; Stellar mass; Redshift; Galaxy; Astronomy; Initial mass function; Extinction (optical mineralogy); Luminous infrared galaxy","score_opus":0.008060992287360276,"score_gpt":0.20455396325589495,"score_spread":0.19649297096853469,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086328762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986488,0.000052801788,0.00009483028,0.000025015694,0.0000016585728,0.0000023294042,0.00020017603,0.000011253681,0.00096312567],"genre_scores_gemma":[0.99915326,0.00003259037,0.00011567565,0.000015639775,0.000005180417,0.0000015799303,0.0003680149,0.000004808437,0.00030325714],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999908,0.000006980444,0.0000020981913,0.000025941037,0.000013221844,0.00004371941],"domain_scores_gemma":[0.99961543,0.000038922586,0.00013103042,0.000043716747,0.000037440594,0.00013338432],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022274021,0.00021671962,0.0002307706,0.00071943767,0.00034469675,0.0009924102,0.00028270143,0.00031087268,0.0009260098],"category_scores_gemma":[0.000460495,0.00015512534,0.0002358795,0.0005687738,0.00036368438,0.00036620448,0.00041012286,0.00048995565,0.00027960064],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021497087,0.000052057047,0.981146,0.000011788979,0.000036706297,0.0002472547,0.00073315063,0.00034538258,0.0124911545,0.0006800837,0.00031829468,0.0037231466],"study_design_scores_gemma":[0.0000017830241,0.000024142853,0.9984573,0.0000015964918,0.000005130133,0.000040177907,0.00012607293,0.0001624165,0.0007443274,0.000060284627,0.0003747008,0.0000019916486],"about_ca_topic_score_codex":0.013857665,"about_ca_topic_score_gemma":0.014126624,"teacher_disagreement_score":0.013857665,"about_ca_system_score_codex":0.00041179155,"about_ca_system_score_gemma":0.00014620289,"threshold_uncertainty_score":0.027553976},"labels":[],"label_agreement":null},{"id":"W2086346033","doi":"10.1086/375510","title":"Cosmological Parameters from Cosmic Background Imager Observations and Comparisons with BOOMERANG, DASI, and MAXIMA","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":218,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Physics; Astrophysics; Maxima; Reionization; Spectral density; COSMIC cancer database; Cosmology; Decoupling (probability); Cosmic background radiation; Galaxy; Cosmic variance; Baryon; Spectral index; Astronomy; Spectral line; Redshift; Statistics; Quantum mechanics","score_opus":0.02708665521789297,"score_gpt":0.24839465115185952,"score_spread":0.22130799593396655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086346033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9880614,0.0001860893,0.0011761823,0.000055331417,0.0000038552935,0.000010418052,0.0024472598,0.0000855861,0.007973725],"genre_scores_gemma":[0.99284464,0.000116231684,0.0018297439,0.000014685629,0.000007630016,0.000011092444,0.0048206844,0.000051983414,0.00030333298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978095,0.000031550866,0.000009902296,0.000060054128,0.000083891755,0.00003367064],"domain_scores_gemma":[0.9993,0.00012772564,0.00024462413,0.00010588777,0.00010378437,0.00011806271],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055587187,0.00034381176,0.0002482971,0.0025395462,0.0003374041,0.0005557352,0.00024220305,0.0001562828,0.00092268287],"category_scores_gemma":[0.0017267655,0.00023705188,0.00027183228,0.001927851,0.00031419285,0.00036487935,0.00043008558,0.00037949163,0.0003178062],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028840775,0.000047043126,0.9463362,0.00005642403,0.00015202834,0.00016801848,0.0005896423,0.0021459681,0.013025948,0.0018156591,0.001502553,0.033872135],"study_design_scores_gemma":[0.000005157324,0.000011827353,0.99522686,0.000004833251,0.000018100829,0.000111218,0.000056882553,0.0010609501,0.0016608988,0.00023585529,0.0015978962,0.000009661842],"about_ca_topic_score_codex":0.008393326,"about_ca_topic_score_gemma":0.020177446,"teacher_disagreement_score":0.008393326,"about_ca_system_score_codex":0.0005557585,"about_ca_system_score_gemma":0.0001616404,"threshold_uncertainty_score":0.016688943},"labels":[],"label_agreement":null},{"id":"W2086461081","doi":"10.1088/0004-637x/769/2/145","title":"THE ACS VIRGO CLUSTER SURVEY. XVII. THE SPATIAL ALIGNMENT OF GLOBULAR CLUSTER SYSTEMS WITH EARLY-TYPE HOST GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Virgo Cluster; Cluster (spacecraft); Galaxy; Galaxy cluster; Host (biology); Elliptical galaxy","score_opus":0.006610109886738916,"score_gpt":0.19575897264126155,"score_spread":0.18914886275452264,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086461081","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01972208,0.0022098576,0.00028701243,0.00089301175,0.0003736999,0.0001997797,0.9647937,0.0005010792,0.011019943],"genre_scores_gemma":[0.043038238,0.001573171,0.0015832959,0.0003810837,0.00018960425,0.0002956806,0.9441323,0.00014355358,0.008663006],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99950254,0.000048314756,0.000056754197,0.00008303125,0.0002005102,0.00010891169],"domain_scores_gemma":[0.9972531,0.00012933923,0.0005749383,0.00025740042,0.0011926582,0.00059259514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001118769,0.0010752442,0.0006909308,0.011437032,0.00089113606,0.0015722421,0.0015372729,0.0006761196,0.011217661],"category_scores_gemma":[0.0029667134,0.0006002869,0.00046650774,0.015388524,0.00032833687,0.0010351668,0.0018553644,0.0010957124,0.0076859235],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017121268,0.000080706945,0.080673136,0.0005480232,0.00016195874,0.000100240664,0.0002257214,0.00027119467,0.00083823607,0.0010797209,0.8884559,0.027393999],"study_design_scores_gemma":[0.00010281797,0.000029475883,0.76637065,0.00017326747,0.000070233014,0.00008629602,0.00032389324,0.00014479441,0.00026531558,0.0005358439,0.23187068,0.000026801392],"about_ca_topic_score_codex":0.22204594,"about_ca_topic_score_gemma":0.24004821,"teacher_disagreement_score":0.22204594,"about_ca_system_score_codex":0.002107262,"about_ca_system_score_gemma":0.002683722,"threshold_uncertainty_score":0.44150704},"labels":[],"label_agreement":null},{"id":"W2086476526","doi":"10.1086/510577","title":"The Cool ISM in Elliptical Galaxies. I. A Survey of Molecular Gas","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Astrophysics; Physics; Elliptical galaxy; Galaxy; Supermassive black hole; Astronomy","score_opus":0.008185763764828225,"score_gpt":0.22575409495786308,"score_spread":0.21756833119303487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086476526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99818593,0.0010213354,0.00012134864,0.000032318072,0.0000017034351,0.0000029655926,0.0001356188,0.000006111585,0.00049262575],"genre_scores_gemma":[0.99914634,0.00034112367,0.00013785469,0.000034073757,0.000009305728,0.0000025804381,0.00018246658,0.0000013921322,0.0001449362],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987805,0.00001954225,0.00000708161,0.000034044315,0.00001973386,0.00004158332],"domain_scores_gemma":[0.999574,0.00004887602,0.00020030054,0.000027384065,0.000032153548,0.000117271076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025696724,0.00018437978,0.00018555702,0.0014068433,0.00029470498,0.0005705236,0.00018945421,0.00021887869,0.0008029902],"category_scores_gemma":[0.0003998341,0.00012988262,0.00013239903,0.00064555847,0.00049269636,0.0004411116,0.00068109063,0.00017153703,0.00023300362],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012001985,0.000024918294,0.97187364,0.000034157052,0.000017181157,0.0000967337,0.0004297244,0.000038326605,0.022339616,0.00016686785,0.00008029913,0.004778501],"study_design_scores_gemma":[9.986345e-7,0.00002751845,0.99890816,0.0000044787334,0.0000058719097,0.00013519541,0.00014956795,0.00003067719,0.00038435878,0.00005660729,0.0002955847,0.0000010101325],"about_ca_topic_score_codex":0.002066519,"about_ca_topic_score_gemma":0.0036023841,"teacher_disagreement_score":0.002066519,"about_ca_system_score_codex":0.00017478966,"about_ca_system_score_gemma":0.00008150953,"threshold_uncertainty_score":0.004108906},"labels":[],"label_agreement":null},{"id":"W2086482471","doi":"10.1086/525246","title":"A Model for Dark Matter Halos","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Galaxy rotation curve; Dark matter; Galaxy; Dark matter halo; Cold dark matter; Adiabatic process; Milky Way; Cuspy halo problem; Halo","score_opus":0.01476526446323639,"score_gpt":0.2177691471258751,"score_spread":0.20300388266263872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086482471","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.25965303,0.007224971,0.57214826,0.008796501,0.0008284797,0.00036534478,0.0023364113,0.0019210053,0.14672595],"genre_scores_gemma":[0.8900006,0.0031407184,0.044439886,0.0006614435,0.00036726386,0.00034348897,0.00064887496,0.00020293545,0.06019483],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997838,0.00007772901,0.000010018695,0.000029676941,0.000038934933,0.00005983997],"domain_scores_gemma":[0.99949217,0.00012809751,0.000054972454,0.00007027705,0.000079991616,0.00017461897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006037724,0.00075907755,0.00067657203,0.0008866603,0.0009922141,0.0022104522,0.0019728548,0.0013622215,0.009427241],"category_scores_gemma":[0.0012177089,0.00035306695,0.0009779516,0.0007608649,0.0011695159,0.0022212954,0.001586428,0.0012361258,0.001863871],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008310456,0.000038136022,0.0012739346,0.00008217648,0.00004987032,0.00056563615,0.00027829866,0.124839,0.0011476318,0.8601943,0.004490815,0.0069571114],"study_design_scores_gemma":[0.00011152015,0.00006918384,0.00051395886,0.000040278872,0.000030323788,0.00045434767,0.00010677802,0.45741495,0.00019372968,0.51654977,0.024481766,0.000033403092],"about_ca_topic_score_codex":0.0052294447,"about_ca_topic_score_gemma":0.0030699214,"teacher_disagreement_score":0.009427241,"about_ca_system_score_codex":0.0012259376,"about_ca_system_score_gemma":0.00077902037,"threshold_uncertainty_score":0.031537294},"labels":[],"label_agreement":null},{"id":"W2086507817","doi":"10.1088/0004-637x/795/2/133","title":"DEEP THERMAL INFRARED IMAGING OF HR 8799 bcde: NEW ATMOSPHERIC CONSTRAINTS AND LIMITS ON A FIFTH PLANET","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planet; Photometry (optics); Planetary mass; Brown dwarf; Atmosphere (unit); Giant planet","score_opus":0.0071318121470150785,"score_gpt":0.20462197920145522,"score_spread":0.19749016705444014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086507817","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937656,0.0001325653,0.0007732617,0.000059371578,0.0000037436093,0.000005258392,0.00045193988,0.00006372332,0.004744617],"genre_scores_gemma":[0.99735546,0.00004219988,0.0015868662,0.000041040315,0.000008011739,0.0000042661604,0.0006164557,0.000011462964,0.00033427437],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999894,0.000007095108,0.000004371073,0.00002652276,0.000039527127,0.000028347024],"domain_scores_gemma":[0.9996412,0.000045247936,0.000097988646,0.00006235545,0.000063585845,0.000089633904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001876127,0.00013645129,0.00013800725,0.00068726664,0.00032029676,0.00048561595,0.00031845857,0.000300155,0.0008529124],"category_scores_gemma":[0.00031983628,0.00014211373,0.00012934141,0.0004387761,0.0001913709,0.00020584169,0.00030131792,0.00035552893,0.00045574273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004398835,0.00016610695,0.7374891,0.00006797664,0.000065070206,0.00085038814,0.000524269,0.0010448243,0.22381648,0.0007413685,0.002726098,0.0320685],"study_design_scores_gemma":[0.000011277305,0.000046212175,0.98526394,0.0000104446435,0.00002009266,0.00047432006,0.00012446233,0.002018002,0.009209647,0.00013335817,0.0026807338,0.0000074050263],"about_ca_topic_score_codex":0.0032679944,"about_ca_topic_score_gemma":0.008371808,"teacher_disagreement_score":0.0032679944,"about_ca_system_score_codex":0.0002866955,"about_ca_system_score_gemma":0.00012157817,"threshold_uncertainty_score":0.006497979},"labels":[],"label_agreement":null},{"id":"W2086603264","doi":"10.1086/429715","title":"On the Interpretation of High‐Velocity White Dwarfs as Members of the Galactic Halo","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Halo; Physics; Galactic halo; Astrophysics; Proper motion; Photometry (optics); Parallax; Astronomy; Population; Stars; Galaxy; Medicine","score_opus":0.007113746456068862,"score_gpt":0.21815357985186976,"score_spread":0.2110398333958009,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086603264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961482,0.00042938464,0.0009896201,0.00005432071,0.0000039657807,0.000010437506,0.00007622495,0.000017170243,0.0022706205],"genre_scores_gemma":[0.99801445,0.00035459423,0.00077159994,0.000030812986,0.000013338136,0.0000044484523,0.00019955687,0.0000039270108,0.00060727686],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998603,0.00003915456,0.000008829294,0.00001625823,0.000042461197,0.00003302542],"domain_scores_gemma":[0.9995036,0.00017319647,0.00011040538,0.000068684705,0.00006325698,0.00008080134],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050877105,0.0003220445,0.00016441419,0.0018655013,0.00051934744,0.0007345151,0.0002776678,0.00016988082,0.0014233658],"category_scores_gemma":[0.0010818487,0.00009322742,0.00016739733,0.0007035519,0.00048927474,0.0003501257,0.0005346977,0.00014231578,0.0005363157],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024916016,0.000028796978,0.94698435,0.00005532825,0.000039350554,0.0020105564,0.000923064,0.0011240295,0.012787537,0.0027009158,0.00048815325,0.03260867],"study_design_scores_gemma":[0.000014494273,0.00016456423,0.9803227,0.00001842286,0.000061080806,0.0045913877,0.0011501316,0.002377547,0.0030298275,0.003004406,0.005251269,0.000014046268],"about_ca_topic_score_codex":0.004432894,"about_ca_topic_score_gemma":0.008580068,"teacher_disagreement_score":0.004432894,"about_ca_system_score_codex":0.00025082016,"about_ca_system_score_gemma":0.00025452257,"threshold_uncertainty_score":0.008814156},"labels":[],"label_agreement":null},{"id":"W2086619535","doi":"10.1088/0004-637x/775/1/56","title":"STIS CORONAGRAPHIC IMAGING OF FOMALHAUT: MAIN BELT STRUCTURE AND THE ORBIT OF FOMALHAUT<i>b</i>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Orbit (dynamics); Orbital eccentricity; Eccentricity (behavior); Planet; Astronomy; RADIUS","score_opus":0.0038249657238203436,"score_gpt":0.18829900372753003,"score_spread":0.18447403800370968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086619535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99508375,0.00012447136,0.00027419906,0.00005183797,0.000006370864,0.0000064051014,0.0017771623,0.00010687056,0.002568962],"genre_scores_gemma":[0.9944997,0.00007058415,0.0013987351,0.000029487,0.000017868302,0.000004122176,0.0034282398,0.00002374756,0.00052740006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994195,0.0000023228176,0.000002997796,0.000015148003,0.000017420783,0.00002024693],"domain_scores_gemma":[0.9997156,0.000014176938,0.00009648209,0.000027267331,0.00005509345,0.00009129881],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010956446,0.00013144301,0.00011087201,0.0009817525,0.00022136362,0.0003653362,0.00017272531,0.00022152069,0.0015281934],"category_scores_gemma":[0.00031541946,0.00008354263,0.00013948996,0.00064791425,0.00013193022,0.00024762072,0.0002758035,0.00019449578,0.00034731269],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047235808,0.00009631965,0.83727163,0.00011973132,0.00009573948,0.0006203028,0.0006727043,0.00075244025,0.11743228,0.00027812787,0.0050421753,0.037146214],"study_design_scores_gemma":[0.0000028391607,0.00001655197,0.9952689,0.0000043671207,0.000008861762,0.00021102134,0.00005468653,0.0004695807,0.0016861698,0.000024203442,0.0022497054,0.000003068536],"about_ca_topic_score_codex":0.013165171,"about_ca_topic_score_gemma":0.03414257,"teacher_disagreement_score":0.013165171,"about_ca_system_score_codex":0.00048670935,"about_ca_system_score_gemma":0.00019671218,"threshold_uncertainty_score":0.026177108},"labels":[],"label_agreement":null},{"id":"W2086624465","doi":"10.1086/323025","title":"The Influence of Stellar Wind Variability on Measurements of Interstellar O [CSC]vi[/CSC] along Sight Lines to Early-Type Stars","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Stars; Astrophysics; Galaxy; Interstellar medium; Large Magellanic Cloud; Astronomy; O-type star","score_opus":0.01868386230298376,"score_gpt":0.22865095530769708,"score_spread":0.20996709300471333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086624465","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978796,0.00009324697,0.0013952561,0.000009231573,0.000004059296,0.0000050443073,0.00019488514,0.000022462213,0.00039621006],"genre_scores_gemma":[0.99812883,0.000040739338,0.0011353173,0.000012529375,0.000007838126,0.0000067856818,0.00054574455,0.000014217006,0.00010807216],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989165,0.00033320938,0.00009289885,0.000285045,0.0002818007,0.00009062473],"domain_scores_gemma":[0.99526215,0.0020751636,0.001348213,0.000537123,0.00058595545,0.00019141193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014667489,0.0002718885,0.00020524983,0.00051037513,0.00031977045,0.0005015707,0.00033470333,0.0002914637,0.00027639864],"category_scores_gemma":[0.0052438937,0.00021421492,0.00020446733,0.0005717809,0.00023000398,0.00033810284,0.0005080713,0.00019444514,0.000161873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010898115,0.000021187976,0.9767957,0.000016881175,0.00009264444,0.00007006467,0.00008590711,0.0012506916,0.014955607,0.00002529765,0.000054065316,0.0065229717],"study_design_scores_gemma":[0.0000016875686,0.000058530823,0.9945327,0.000003575637,0.000024957912,0.00013681214,0.00003243762,0.0018757122,0.0031301565,0.000017796092,0.00018085659,0.000004729831],"about_ca_topic_score_codex":0.0051027853,"about_ca_topic_score_gemma":0.011971031,"teacher_disagreement_score":0.0051027853,"about_ca_system_score_codex":0.00023321854,"about_ca_system_score_gemma":0.00017210864,"threshold_uncertainty_score":0.010146141},"labels":[],"label_agreement":null},{"id":"W2086649316","doi":"10.1086/318898","title":"Tidal Stirring and the Origin of Dwarf Spheroidals in the Local Group","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":271,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Dark matter; Dwarf galaxy; Astronomy; Dark matter halo; Local Group; Galaxy; Cuspy halo problem; Halo; Milky Way","score_opus":0.008490712640168738,"score_gpt":0.21881156365686005,"score_spread":0.21032085101669132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086649316","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99501723,0.000051338997,0.00086534326,0.00008550231,0.000013276499,0.000013895684,0.00020925635,0.00009787307,0.003646215],"genre_scores_gemma":[0.9986902,0.000026293174,0.0006330911,0.000019733923,0.0000049051546,0.000008582157,0.00021797756,0.000027738597,0.00037142937],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992955,0.00001723174,0.0000034249783,0.000011543649,0.000011779693,0.000026394637],"domain_scores_gemma":[0.99920684,0.00026439968,0.00013276326,0.00005965796,0.000081572005,0.0002546777],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003319014,0.0004017448,0.00037441996,0.0005181039,0.000646796,0.00078732974,0.00072083704,0.0007006186,0.0017573234],"category_scores_gemma":[0.0018090663,0.0002562746,0.00045739263,0.00043095025,0.00064291956,0.000431727,0.0005940531,0.000513366,0.00025880735],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026077157,0.00019977526,0.05910568,0.00004734081,0.00008571586,0.00048396798,0.00018729387,0.9293268,0.0031459152,0.0030998639,0.0009582923,0.0030986092],"study_design_scores_gemma":[0.000054065196,0.00004441276,0.0066355253,0.000005271925,0.000013468022,0.000024794717,0.000075855765,0.9919601,0.0003263759,0.00056387624,0.00028846943,0.000007705432],"about_ca_topic_score_codex":0.023616588,"about_ca_topic_score_gemma":0.013979163,"teacher_disagreement_score":0.023616588,"about_ca_system_score_codex":0.0009631861,"about_ca_system_score_gemma":0.0006345644,"threshold_uncertainty_score":0.046958208},"labels":[],"label_agreement":null},{"id":"W2086667163","doi":"10.1086/308366","title":"Further Evidence for Carbon Isotopic Structure in the λλ5797 and 6614 Diffuse Interstellar Bands","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Stars; Interstellar medium; Spectral line; Wavelength; Astronomy; Optics; Galaxy","score_opus":0.014833351610351219,"score_gpt":0.25543173516697876,"score_spread":0.24059838355662755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086667163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981053,0.00009331922,0.00029711536,0.000017505488,0.000002296595,0.000002366139,0.00012876885,0.000012090825,0.001341291],"genre_scores_gemma":[0.9987093,0.00004950744,0.0003542783,0.0000190579,0.0000031687946,0.000003519337,0.00039468796,0.000008486363,0.00045792817],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988115,0.000005850367,0.000007330667,0.000041832005,0.000035337453,0.000028527547],"domain_scores_gemma":[0.99940336,0.00009785609,0.00018445741,0.00007303809,0.00010186949,0.00013951077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018058778,0.00025058948,0.00028278393,0.0010005025,0.00042922606,0.00042851962,0.000310785,0.0003634653,0.003474207],"category_scores_gemma":[0.0005104038,0.00022103397,0.00026019686,0.0012012612,0.00043260408,0.000216249,0.00052113505,0.00029437643,0.0005061262],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006041353,0.00013175615,0.6269963,0.00011465932,0.00016131082,0.00053145,0.0007028834,0.00071032357,0.35140592,0.0011995957,0.00032251197,0.017119141],"study_design_scores_gemma":[0.00001947836,0.00004269138,0.98921573,0.000009806037,0.000026977961,0.00028201207,0.0001859861,0.0010816933,0.008026213,0.00024026398,0.00086183375,0.0000073261667],"about_ca_topic_score_codex":0.0028320649,"about_ca_topic_score_gemma":0.003566003,"teacher_disagreement_score":0.003474207,"about_ca_system_score_codex":0.00026129195,"about_ca_system_score_gemma":0.00019829647,"threshold_uncertainty_score":0.011622369},"labels":[],"label_agreement":null},{"id":"W2086727759","doi":"10.1086/427203","title":"Supernova Simulations with Boltzmann Neutrino Transport: A Comparison of Methods","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":316,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Neutrino; Boltzmann equation; Supernova; Gravitational collapse; Astrophysics; Classical mechanics; Nuclear physics; Quantum mechanics","score_opus":0.039076965390578845,"score_gpt":0.38077652605341644,"score_spread":0.3416995606628376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086727759","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5192959,0.0021087301,0.44453526,0.00074011815,0.00042157373,0.00069675065,0.0012058925,0.0056286864,0.025367126],"genre_scores_gemma":[0.76265174,0.0014896386,0.22900845,0.00017261325,0.00007305671,0.0007270509,0.00070779864,0.0015131193,0.0036563906],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99914813,0.00030544781,0.00009551801,0.000072658026,0.00030110803,0.00007712795],"domain_scores_gemma":[0.99782,0.001032263,0.00016164458,0.0003872297,0.00043386617,0.00016507372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013928342,0.00084550364,0.0010780216,0.00077944185,0.00072504964,0.0011839579,0.0021346575,0.001159359,0.0019147103],"category_scores_gemma":[0.005340431,0.0006094591,0.00078348356,0.0010646397,0.0005865848,0.0013012642,0.001408362,0.0012157272,0.00045380366],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005438868,0.0002579864,0.0060683037,0.00025162037,0.00018969011,0.000119751676,0.00042726516,0.9233692,0.00558396,0.022351788,0.00056515244,0.04027126],"study_design_scores_gemma":[0.00009356015,0.00004150645,0.00035960946,0.000014891906,0.000012392595,0.000022781518,0.000042409418,0.9944404,0.0018365959,0.0020882683,0.0010254921,0.000022047632],"about_ca_topic_score_codex":0.017159121,"about_ca_topic_score_gemma":0.007696758,"teacher_disagreement_score":0.017159121,"about_ca_system_score_codex":0.0013160707,"about_ca_system_score_gemma":0.0020195376,"threshold_uncertainty_score":0.034118533},"labels":[],"label_agreement":null},{"id":"W2086745322","doi":"10.1086/381156","title":"On the Properties of Galactic Novae and Their Orbital Period Distribution","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Physics; Astrophysics; Orbital period; Population; Degenerate energy levels; Astronomy; Stars; Range (aeronautics); Nova (rocket); White dwarf","score_opus":0.014651751969769854,"score_gpt":0.20244993651591298,"score_spread":0.1877981845461431,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086745322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870952,0.00024106906,0.00888788,0.000024510588,0.0000047633544,0.00001416701,0.00060271955,0.00005781113,0.0030719223],"genre_scores_gemma":[0.99632543,0.00017352044,0.0021186867,0.000006448203,0.000009470529,0.000016808051,0.0009621338,0.000021204674,0.00036634007],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982196,0.000035308618,0.00001119198,0.00006861478,0.000035450255,0.000027485898],"domain_scores_gemma":[0.9979594,0.0011225377,0.00045722068,0.00017654388,0.00018794433,0.00009640946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006363923,0.0001427002,0.00020945567,0.001735898,0.0002796449,0.00066045753,0.0001892437,0.0001648171,0.0016481847],"category_scores_gemma":[0.0038201222,0.00013376561,0.00031591332,0.0009705501,0.00024040598,0.00037876496,0.00028679802,0.00024618075,0.00030703505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011735746,0.000029018103,0.9158517,0.000046889265,0.00012256148,0.00015239269,0.00027175638,0.020106716,0.019128729,0.0055235527,0.00028550043,0.038363874],"study_design_scores_gemma":[0.000007460735,0.000067050314,0.92010546,0.000012417453,0.00003138931,0.00064180826,0.00014000323,0.0709741,0.0036860837,0.0026831345,0.0016337682,0.000017437056],"about_ca_topic_score_codex":0.0012475877,"about_ca_topic_score_gemma":0.0011442509,"teacher_disagreement_score":0.001735898,"about_ca_system_score_codex":0.00025476242,"about_ca_system_score_gemma":0.00011689715,"threshold_uncertainty_score":0.0055137277},"labels":[],"label_agreement":null},{"id":"W2086772437","doi":"10.1086/425857","title":"Pulse Shapes from Rapidly Rotating Neutron Stars: Equatorial Photon Orbits","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; University of Alberta","funders":"","keywords":"Neutron star; Pulsar; RADIUS; Schwarzschild radius; Pulse (music); Light curve; Millisecond pulsar; Photon; Flux (metallurgy)","score_opus":0.014432219860562825,"score_gpt":0.2360700639405417,"score_spread":0.22163784407997889,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086772437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83995813,0.0004897108,0.1494609,0.00019729462,0.000060143808,0.00006832386,0.0008695521,0.0010567921,0.007839166],"genre_scores_gemma":[0.97087413,0.00027414897,0.026338264,0.00002583205,0.000026001006,0.000038822087,0.0010955705,0.00024849418,0.0010787174],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99980766,0.000047043613,0.00001289953,0.000028146267,0.00008027368,0.000023989154],"domain_scores_gemma":[0.9982002,0.00082429213,0.00033992715,0.00022416511,0.00031698233,0.000094360694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009065251,0.00045697097,0.00034606436,0.00089886173,0.00033049885,0.0006117515,0.00066886743,0.0004913667,0.0012638952],"category_scores_gemma":[0.0040870663,0.00026830373,0.00053389353,0.0011808381,0.00030373866,0.0004243855,0.000712665,0.0009344612,0.0003971003],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00144198,0.000113472,0.051136557,0.00089308416,0.0002344493,0.0021453642,0.0027917547,0.6762407,0.11302987,0.03426352,0.0028000576,0.114909224],"study_design_scores_gemma":[0.00005504857,0.0002561143,0.034829203,0.000085382955,0.000055517216,0.0008067364,0.00022991351,0.8852316,0.06426711,0.0099423,0.0041244817,0.000116495605],"about_ca_topic_score_codex":0.0012813146,"about_ca_topic_score_gemma":0.0009464506,"teacher_disagreement_score":0.0012813146,"about_ca_system_score_codex":0.00055236387,"about_ca_system_score_gemma":0.00030939464,"threshold_uncertainty_score":0.00479424},"labels":[],"label_agreement":null},{"id":"W2086779960","doi":"10.1086/308642","title":"The Globular Cluster Systems in the Coma Ellipticals. I. The Luminosity Function in NGC 4874 and Implications for Hubble’s Constant","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Queen's University; Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Globular cluster; Astrophysics; Physics; Coma Cluster; Virgo Cluster; Galaxy; Astronomy; Fornax Cluster; Elliptical galaxy; Coma (optics); Hubble's law; Velocity dispersion; Advanced Camera for Surveys; Distance modulus; Galaxy cluster; Hubble space telescope; Redshift","score_opus":0.008646540683425944,"score_gpt":0.21869331771293005,"score_spread":0.2100467770295041,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086779960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99891376,0.00010161364,0.000056204753,0.000025559371,7.708684e-7,0.0000013305864,0.00004699555,0.000004830446,0.00084895466],"genre_scores_gemma":[0.99973553,0.000030688865,0.000054272517,0.0000053769977,0.0000011777109,9.851815e-7,0.000039361228,6.6701415e-7,0.0001319131],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990404,0.00001173348,0.0000037650027,0.000014862046,0.000018338038,0.00004718205],"domain_scores_gemma":[0.9996195,0.00003622498,0.00014284188,0.000032613974,0.00005723292,0.00011155196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016971664,0.00011592266,0.00010119727,0.0010417744,0.00058789,0.00052435615,0.00021520964,0.00015069681,0.0011771214],"category_scores_gemma":[0.0005408754,0.00009274788,0.000077179735,0.00059490424,0.00069495157,0.00036853307,0.0004956744,0.00014837131,0.00016467337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018064522,0.000025121146,0.96598613,0.000016802158,0.00001977919,0.00039906192,0.0014228115,0.00053558435,0.015760034,0.0034452097,0.00043520785,0.01177363],"study_design_scores_gemma":[0.0000021949743,0.000015155597,0.9979467,0.0000029575283,0.000003515486,0.00009474173,0.0002785576,0.0002718724,0.00048645004,0.00035519563,0.00053987594,0.0000027450426],"about_ca_topic_score_codex":0.02671356,"about_ca_topic_score_gemma":0.034671593,"teacher_disagreement_score":0.02671356,"about_ca_system_score_codex":0.0010472958,"about_ca_system_score_gemma":0.00017307102,"threshold_uncertainty_score":0.053116143},"labels":[],"label_agreement":null},{"id":"W2086837267","doi":"10.1086/341811","title":"Shapes of Molecular Cloud Cores and the Filamentary Mode of Star Formation","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Prolate spheroid; Molecular cloud; Oblate spheroid; Monte Carlo method; Gaussian; Star formation; Flux (metallurgy); Mass distribution; Core (optical fiber)","score_opus":0.009075556661221148,"score_gpt":0.22124513326546563,"score_spread":0.2121695766042445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086837267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978174,0.000022091343,0.0014739907,0.000013575212,0.0000011332971,0.000007646339,0.00015020293,0.00002039119,0.00049342215],"genre_scores_gemma":[0.9986279,0.000014254451,0.0010256404,0.0000029929201,0.0000011461766,0.0000052002733,0.0002399237,0.000008956435,0.00007391041],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999325,0.000013914065,0.0000036138126,0.00002042247,0.000013716897,0.0000157992],"domain_scores_gemma":[0.9992442,0.00029290424,0.0002217626,0.000067090994,0.00009456827,0.00007944408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027904086,0.00014655686,0.000092640934,0.0005347117,0.00023662104,0.00037593444,0.00035323697,0.00027447063,0.00056289014],"category_scores_gemma":[0.0019506903,0.00017406682,0.00022835989,0.0002951169,0.0002833693,0.00019465885,0.00018989513,0.00018616025,0.000099938225],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042956465,0.00016211747,0.5171905,0.000048953294,0.00007212734,0.0006319402,0.0004483833,0.42347386,0.03705172,0.0072703105,0.00055737584,0.012663191],"study_design_scores_gemma":[0.00006138671,0.00012498288,0.2275873,0.000013438076,0.000032956606,0.0006108995,0.00008069177,0.75398594,0.013820441,0.002800923,0.0008501149,0.00003094115],"about_ca_topic_score_codex":0.0021972354,"about_ca_topic_score_gemma":0.002968693,"teacher_disagreement_score":0.0021972354,"about_ca_system_score_codex":0.00061456393,"about_ca_system_score_gemma":0.0001530706,"threshold_uncertainty_score":0.0044590235},"labels":[],"label_agreement":null},{"id":"W2086866159","doi":"10.1088/0004-637x/738/1/58","title":"EXTENDED STAR CLUSTERS IN THE REMOTE HALO OF THE INTRIGUING DWARF GALAXY NGC 6822","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Globular cluster; Star cluster; Dwarf galaxy; Irregular galaxy; Galaxy; Halo; Star formation; Galactic halo; Local Group","score_opus":0.014533955794535312,"score_gpt":0.21781357594937328,"score_spread":0.20327962015483797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086866159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965465,0.00011639937,0.00002122015,0.000005767011,4.8305606e-7,7.641057e-7,0.000030591833,0.0000020097798,0.0001681375],"genre_scores_gemma":[0.999387,0.00014950612,0.00010050719,0.0000047682306,0.0000042030674,0.0000013108096,0.00019032793,0.0000013220885,0.00016105254],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992406,0.000010005167,0.0000038128433,0.000019472418,0.000018760082,0.000023971088],"domain_scores_gemma":[0.99977714,0.000018517556,0.00007261922,0.000015027844,0.000023385983,0.00009334618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000078892175,0.00019530972,0.00015418125,0.0008419184,0.00036730355,0.0005126709,0.00014208391,0.0001367725,0.000463929],"category_scores_gemma":[0.00021615316,0.00008755475,0.000106893065,0.0008918207,0.00024819034,0.00022619075,0.00047016604,0.00007927188,0.00009947795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012175063,0.00003670775,0.96966404,0.00003585964,0.000057068868,0.0012697214,0.0015620603,0.0005873618,0.017429683,0.00035109924,0.00023810781,0.008646601],"study_design_scores_gemma":[0.0000050439035,0.000041353636,0.9964855,0.000003793768,0.000017604665,0.0005780529,0.0006533384,0.00023653335,0.00031307378,0.000074449745,0.0015870265,0.0000042857337],"about_ca_topic_score_codex":0.009097077,"about_ca_topic_score_gemma":0.01821549,"teacher_disagreement_score":0.009097077,"about_ca_system_score_codex":0.0002596019,"about_ca_system_score_gemma":0.0001614223,"threshold_uncertainty_score":0.018088222},"labels":[],"label_agreement":null},{"id":"W2086929564","doi":"10.1086/505519","title":"Cepheid Masses:<i>FUSE</i>Observations of S Muscae","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Cepheid variable; Astrophysics; Physics; Spectral line; Flux (metallurgy); Effective temperature; Amplitude; Stars; Fuse (electrical); Astronomy; Materials science; Optics","score_opus":0.013739940047896318,"score_gpt":0.21673276428544525,"score_spread":0.20299282423754894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2086929564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9339365,0.0005926134,0.0028626635,0.00017614078,0.00004994664,0.000029766648,0.016648438,0.0005769175,0.045127016],"genre_scores_gemma":[0.9831739,0.00015757348,0.003421738,0.000051903677,0.000030382625,0.000013255995,0.008607939,0.000041717707,0.004501669],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999931,0.000005533727,0.00000423092,0.000018707933,0.00002966221,0.000010934264],"domain_scores_gemma":[0.99987304,0.000011892454,0.00005392274,0.000019379018,0.000021128795,0.000020687767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009804778,0.00025862607,0.00011825927,0.0009835454,0.00036056648,0.00025378252,0.000346824,0.00019296003,0.0075600417],"category_scores_gemma":[0.00032088085,0.000062271836,0.000103004546,0.0006100819,0.00012983693,0.0003842571,0.00033674712,0.00018121375,0.0017224705],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008550718,0.00016300558,0.69100875,0.0002499029,0.00020159334,0.0013933966,0.0012565122,0.0023307633,0.16113406,0.006710957,0.04022546,0.094470456],"study_design_scores_gemma":[0.000005998163,0.00006295671,0.966387,0.000008734103,0.000013701182,0.00041631478,0.000063395564,0.0009867067,0.0077656615,0.0005188469,0.02376042,0.000010222368],"about_ca_topic_score_codex":0.0027952697,"about_ca_topic_score_gemma":0.0063518193,"teacher_disagreement_score":0.0075600417,"about_ca_system_score_codex":0.00025257704,"about_ca_system_score_gemma":0.00004467345,"threshold_uncertainty_score":0.025290847},"labels":[],"label_agreement":null},{"id":"W2087024901","doi":"10.1088/0004-637x/796/2/91","title":"THE QUENCHING OF THE ULTRA-FAINT DWARF GALAXIES IN THE REIONIZATION ERA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":328,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Reionization; Galaxy; Dwarf galaxy; Milky Way; Stars; Star formation; Dwarf spheroidal galaxy","score_opus":0.0070251350028837835,"score_gpt":0.24397901333814437,"score_spread":0.23695387833526058,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087024901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97947776,0.0012420329,0.00074119703,0.0008504425,0.00002317278,0.000006993841,0.000315355,0.00010976598,0.01723325],"genre_scores_gemma":[0.9953159,0.00018937048,0.00013504107,0.00014300596,0.00001680693,0.0000054147695,0.00016615805,0.000015505033,0.004012676],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998909,0.000010821046,0.0000025538557,0.00004210747,0.000024111203,0.00002954665],"domain_scores_gemma":[0.9992424,0.00012819614,0.0002196142,0.000082911305,0.00014423119,0.00018252658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024149238,0.00009490702,0.00015585078,0.00073775015,0.00050695764,0.0008059649,0.00025088928,0.0004224199,0.007310414],"category_scores_gemma":[0.0013040061,0.00010717038,0.0001212296,0.000558017,0.0004640622,0.0006173271,0.00058626983,0.0005006345,0.0006638356],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052643253,0.00019586863,0.69283146,0.00016471423,0.00008569672,0.00030521437,0.006311936,0.0009815026,0.13269064,0.017156566,0.008146454,0.14060359],"study_design_scores_gemma":[0.0000042716615,0.00003267025,0.9892462,0.000009123426,0.000008904539,0.00008781359,0.0005026317,0.00032491793,0.0018483866,0.002101858,0.0058263275,0.0000069175817],"about_ca_topic_score_codex":0.008671029,"about_ca_topic_score_gemma":0.009917279,"teacher_disagreement_score":0.008671029,"about_ca_system_score_codex":0.000734869,"about_ca_system_score_gemma":0.00026430842,"threshold_uncertainty_score":0.024455786},"labels":[],"label_agreement":null},{"id":"W2087104895","doi":"10.1086/491667","title":"Afterglows, Redshifts, and Properties of<i>Swift</i>Gamma‐Ray Bursts","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Redshift; Gamma-ray burst; Physics; Afterglow; Astrophysics; Swift; Luminosity; Extinction (optical mineralogy); Brightness; Astronomy; Limiting; Galaxy; Optics","score_opus":0.010342948088041103,"score_gpt":0.20833277331239178,"score_spread":0.19798982522435069,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087104895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99913174,0.000062381645,0.000104401974,0.000007255715,0.0000017180387,0.0000029559758,0.00023178943,0.000011797231,0.00044596955],"genre_scores_gemma":[0.99855,0.00007216675,0.00016985256,0.0000112634325,0.000011245873,0.000004579398,0.0009327238,0.000011341774,0.000236741],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998721,0.0000071542,0.000018434153,0.000035484438,0.00002782073,0.00003897887],"domain_scores_gemma":[0.99859303,0.00015603311,0.0007951494,0.00011475026,0.00018184661,0.0001590452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002499662,0.00018312581,0.00019847315,0.00140546,0.00024332262,0.00061849196,0.00022170877,0.00021324836,0.0006067985],"category_scores_gemma":[0.000955198,0.0001357057,0.00023826986,0.0008501804,0.0002454893,0.00030564252,0.00027307757,0.00025345173,0.00025102159],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015927543,0.000021185444,0.9807709,0.000011022312,0.000029859659,0.00018649068,0.00017519078,0.00018423768,0.011997406,0.000048298964,0.00013620782,0.006280046],"study_design_scores_gemma":[8.9736005e-7,0.0000177486,0.99887866,0.0000015290674,0.000006497418,0.00016234657,0.000027345553,0.00008275356,0.00064973783,0.000010491968,0.00015996821,0.0000019524757],"about_ca_topic_score_codex":0.0030906263,"about_ca_topic_score_gemma":0.00302048,"teacher_disagreement_score":0.0030906263,"about_ca_system_score_codex":0.00020305529,"about_ca_system_score_gemma":0.00007454066,"threshold_uncertainty_score":0.006145239},"labels":[],"label_agreement":null},{"id":"W2087104961","doi":"10.1088/0004-637x/738/2/129","title":"DISCOVERY OF A CANDIDATE QUIESCENT LOW-MASS X-RAY BINARY IN THE GLOBULAR CLUSTER NGC 6553","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Globular cluster; Cluster (spacecraft); Binary number; Neutron star; RADIUS; Spectral line; Star cluster; Luminosity","score_opus":0.013225798097951406,"score_gpt":0.21992328074808792,"score_spread":0.20669748265013652,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087104961","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994492,0.000074418014,0.00009032834,0.0000094410625,0.0000023887233,0.0000038804988,0.00005471621,0.0000084861085,0.00030712],"genre_scores_gemma":[0.9995079,0.000025103967,0.00016550742,0.000010309321,0.0000026198627,0.0000014546341,0.0001497264,0.0000016181411,0.00013568877],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991286,0.0000056487547,0.000006874328,0.000029505763,0.000020353862,0.000024708681],"domain_scores_gemma":[0.9998053,0.000017812943,0.000048990707,0.000020480487,0.000019387577,0.00008809653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016271189,0.00015688733,0.00019890604,0.00083831046,0.0005889132,0.0006310088,0.00025153597,0.0002772456,0.00070760323],"category_scores_gemma":[0.00026879174,0.0000860178,0.00012284888,0.0004927278,0.0002955212,0.0001524405,0.0005120038,0.00010295024,0.00023811271],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028289668,0.00005287341,0.9046995,0.000045978588,0.000039872633,0.002281387,0.0011568367,0.00024415238,0.07864135,0.0005437423,0.0003421335,0.011669395],"study_design_scores_gemma":[0.00000991541,0.00014209855,0.99421376,0.000010558673,0.000027099868,0.00077666645,0.00044423438,0.00052668556,0.0025347888,0.00010062478,0.0012062055,0.0000074303507],"about_ca_topic_score_codex":0.005548041,"about_ca_topic_score_gemma":0.009648353,"teacher_disagreement_score":0.005548041,"about_ca_system_score_codex":0.0003457552,"about_ca_system_score_gemma":0.0001536258,"threshold_uncertainty_score":0.011031449},"labels":[],"label_agreement":null},{"id":"W2087154189","doi":"10.1086/309114","title":"How to Identify Pre‐Protostellar Cores","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Physics; Photometry (optics); Line (geometry); Astronomy; Stars","score_opus":0.011156961077214051,"score_gpt":0.264022436137898,"score_spread":0.25286547506068396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087154189","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8723163,0.006394768,0.08925167,0.0026554964,0.00084584195,0.0011627199,0.0029637865,0.001669,0.022740392],"genre_scores_gemma":[0.7837359,0.0015186747,0.19936131,0.00067690486,0.0002614364,0.0003635614,0.005261078,0.00022104604,0.008600228],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.99961406,0.0000560709,0.000042031304,0.0001064664,0.00007711316,0.00010422858],"domain_scores_gemma":[0.9951108,0.0008015185,0.0004573902,0.00044946175,0.0023975056,0.0007832624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010772147,0.00035927564,0.0006563056,0.0023729932,0.00083992636,0.0027421075,0.0011239642,0.0011659758,0.005925663],"category_scores_gemma":[0.006517042,0.00033011904,0.0003851593,0.0008819372,0.00023562259,0.0017561485,0.0006814337,0.0005357412,0.0051683416],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004852435,0.00028903762,0.5395294,0.0007035225,0.00009469711,0.0010024655,0.0007424866,0.0020844473,0.042806324,0.0025313844,0.020740358,0.3889907],"study_design_scores_gemma":[0.0003781641,0.0004999651,0.764927,0.00092623575,0.00040458495,0.004354475,0.0084086135,0.059229642,0.0636488,0.020996489,0.07601057,0.00021553757],"about_ca_topic_score_codex":0.005989044,"about_ca_topic_score_gemma":0.012062976,"teacher_disagreement_score":0.005989044,"about_ca_system_score_codex":0.00032665307,"about_ca_system_score_gemma":0.0009315676,"threshold_uncertainty_score":0.019823313},"labels":[],"label_agreement":null},{"id":"W2087249160","doi":"10.1086/518030","title":"Spectral and Rotational Changes in the Isolated Neutron Star RX J0720.4-3125","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Neutron star; Glitch; Spectral line; Accretion (finance); Event (particle physics); X-ray binary; Astronomy; Optics","score_opus":0.012563674055307108,"score_gpt":0.23868676783547932,"score_spread":0.2261230937801722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087249160","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873286,0.00008811953,0.00013149017,0.000015429474,0.000004337862,0.0000024765282,0.00015886826,0.000028138275,0.00083832105],"genre_scores_gemma":[0.99795234,0.000064717635,0.00035656014,0.000023345077,0.000012427078,0.000005627355,0.0012093252,0.00003029404,0.00034531005],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989057,0.000009364206,0.0000062601825,0.000034063054,0.000035878533,0.000023752604],"domain_scores_gemma":[0.99963295,0.000034434615,0.000118695854,0.0000414069,0.000060166414,0.000112295944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020984208,0.00034804587,0.00041173678,0.0008572968,0.00035736425,0.00044738472,0.0003097591,0.0003292145,0.0009916495],"category_scores_gemma":[0.00036914437,0.00022065137,0.0003756387,0.0006422055,0.0003429253,0.00020200016,0.00048339867,0.0003894672,0.0003134311],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009472178,0.00033198795,0.38287163,0.00016750589,0.00025119138,0.0014121346,0.00060666003,0.0024808128,0.59045786,0.0006861083,0.0010596,0.018727161],"study_design_scores_gemma":[0.00001767949,0.00010642816,0.99293023,0.0000059897507,0.000027528293,0.00043729064,0.00006269078,0.0013729092,0.0043208147,0.000062068815,0.00064645614,0.00000986658],"about_ca_topic_score_codex":0.001903089,"about_ca_topic_score_gemma":0.004117814,"teacher_disagreement_score":0.001903089,"about_ca_system_score_codex":0.00031655308,"about_ca_system_score_gemma":0.00008112832,"threshold_uncertainty_score":0.0037840605},"labels":[],"label_agreement":null},{"id":"W2087249603","doi":"10.1088/0004-637x/775/1/3","title":"MULTIWAVELENGTH OBSERVATIONS AND MODELING OF 1ES 1959+650 IN A LOW FLUX STATE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; BL Lac object; Flux (metallurgy); Spectral energy distribution; Fermi Gamma-ray Space Telescope; Luminosity; Flare; Light curve; Electron; Synchrotron radiation; Synchrotron; Kinetic energy; Spectral index; Telescope; Blazar; Crab Nebula; Spectral line; Astronomy; Galaxy; Gamma ray; Nuclear physics","score_opus":0.01720341519256062,"score_gpt":0.2209451446978085,"score_spread":0.20374172950524788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087249603","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99762636,0.00006723267,0.0010340054,0.000032625398,0.0000019670547,0.0000068360073,0.00024682772,0.000039172362,0.00094491953],"genre_scores_gemma":[0.99865294,0.00003023017,0.00044200648,0.000009277461,0.0000026771886,0.000004300913,0.00041921853,0.000011357534,0.00042807392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990845,0.000007945273,0.00000537922,0.0000334467,0.000016670336,0.000028118571],"domain_scores_gemma":[0.99986064,0.000020252312,0.00005789536,0.000016739248,0.000015672025,0.00002881279],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002042939,0.00022479112,0.00026554175,0.0008855947,0.0002982853,0.0007555284,0.00072637264,0.0003296803,0.0012098547],"category_scores_gemma":[0.00043156857,0.0003070898,0.00045685866,0.0004429137,0.00029976608,0.00036294974,0.00057012355,0.00030816204,0.0002120337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045870623,0.00024374406,0.74487984,0.00010850076,0.00016388456,0.00093574234,0.00065367663,0.1777081,0.051103078,0.004847998,0.0010722841,0.017824309],"study_design_scores_gemma":[0.00006627987,0.00017568155,0.5802753,0.00002244152,0.00007322491,0.00030577724,0.000212852,0.41139516,0.0039152983,0.0015375235,0.001973359,0.000047220146],"about_ca_topic_score_codex":0.023183148,"about_ca_topic_score_gemma":0.028490119,"teacher_disagreement_score":0.023183148,"about_ca_system_score_codex":0.0017698895,"about_ca_system_score_gemma":0.00032851784,"threshold_uncertainty_score":0.046096385},"labels":[],"label_agreement":null},{"id":"W2087371263","doi":"10.1086/368018","title":"Spatially Resolved 3 Micron Spectroscopy of IRAS 22272+5435: Formation and Evolution of Aliphatic Hydrocarbon Dust in Proto–Planetary Nebulae","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Hydrocarbon; Spectroscopy; Astrophysics; Emission spectrum; Chemistry; Physics; Spectral line; Analytical Chemistry (journal); Astronomy; Organic chemistry","score_opus":0.006887072924293247,"score_gpt":0.21526027992561164,"score_spread":0.2083732070013184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087371263","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99849343,0.00021883767,0.00029423798,0.00002077086,0.000002054819,0.0000020822692,0.00008220967,0.000043747,0.00084263616],"genre_scores_gemma":[0.9987936,0.00005150191,0.0007560763,0.000014319401,0.0000034394793,0.0000024750377,0.00011225206,0.00000450791,0.0002618143],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996364,0.0000019002355,7.5484434e-7,0.000010324689,0.000011536052,0.0000118928965],"domain_scores_gemma":[0.9999511,0.0000052463474,0.000016941378,0.000004532903,0.000008385895,0.000013808886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000050465904,0.00017087751,0.00013134454,0.00031795588,0.00022439218,0.00016111707,0.00019214577,0.00022324984,0.00081655633],"category_scores_gemma":[0.00011477555,0.0001022349,0.00012803882,0.00020602609,0.00013036032,0.000131711,0.00018162892,0.00017904879,0.0001532808],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032413882,0.00011280067,0.10717464,0.0000812262,0.00006973521,0.00069761253,0.0003247888,0.0017875212,0.8699986,0.0005524757,0.00078942574,0.018087188],"study_design_scores_gemma":[0.000016584112,0.00015988313,0.9574586,0.000010683884,0.000052215313,0.0008959735,0.00012975864,0.0032817763,0.035182904,0.00030986645,0.002482659,0.000019132045],"about_ca_topic_score_codex":0.0023426064,"about_ca_topic_score_gemma":0.0049414397,"teacher_disagreement_score":0.0023426064,"about_ca_system_score_codex":0.0002618618,"about_ca_system_score_gemma":0.00008263621,"threshold_uncertainty_score":0.0046578646},"labels":[],"label_agreement":null},{"id":"W2087386595","doi":"10.1086/510193","title":"A Large‐Scale Survey of NGC 1333","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Stars; Star formation; Low Mass; Infrared; Virial theorem; Astronomy; Galaxy","score_opus":0.01363706019635158,"score_gpt":0.2614239049848092,"score_spread":0.24778684478845764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087386595","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978801,0.000043224623,0.00009974974,0.000028750645,0.0000010559802,0.0000090933545,0.00089401833,0.00004170205,0.0010023445],"genre_scores_gemma":[0.9960769,0.000060417293,0.0004949625,0.00003495264,0.000004394816,0.00001777792,0.0026932072,0.000015562473,0.0006017707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983895,0.000015610203,0.000007276885,0.000044131764,0.00004628049,0.000047776466],"domain_scores_gemma":[0.99967575,0.000015697533,0.000099664656,0.00003691093,0.000048368172,0.00012367312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016235931,0.00019118487,0.00018575546,0.000738144,0.00054768025,0.0003316104,0.0002446395,0.0001762003,0.0013615316],"category_scores_gemma":[0.00026391508,0.00011891468,0.00021391938,0.0011074481,0.00023509884,0.00016138415,0.0004336069,0.00019910034,0.00052755384],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013081799,0.00007578107,0.9554408,0.00003967054,0.000066170585,0.00066788634,0.001330881,0.0003847467,0.024054207,0.00018491008,0.0033174693,0.014306667],"study_design_scores_gemma":[0.0000029333692,0.000015418203,0.99751794,0.000002768962,0.0000055784926,0.00017223894,0.0001845489,0.00021889781,0.00024485367,0.000013027224,0.0016186201,0.000003097901],"about_ca_topic_score_codex":0.09079252,"about_ca_topic_score_gemma":0.18510726,"teacher_disagreement_score":0.09079252,"about_ca_system_score_codex":0.0010145869,"about_ca_system_score_gemma":0.0006661964,"threshold_uncertainty_score":0.1805281},"labels":[],"label_agreement":null},{"id":"W2087412056","doi":"10.1086/428923","title":"The Phoenix Deep Survey: Spectroscopic Catalog","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Redshift; Luminosity function; Stars; Galaxy; Luminosity; Astronomy; Active galactic nucleus; Balmer series; Star formation; Population; Extinction (optical mineralogy); Radio galaxy; Emission spectrum; Spectral line; Optics","score_opus":0.007450940178951729,"score_gpt":0.22003848696531694,"score_spread":0.2125875467863652,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087412056","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.24072818,0.0009861783,0.008755674,0.00046721692,0.000040658004,0.000932844,0.7175638,0.0013309695,0.02919451],"genre_scores_gemma":[0.124748655,0.0014803142,0.017551292,0.0004028597,0.00012017911,0.0008101305,0.83847284,0.0002952927,0.016118405],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962234,0.000039620878,0.000030297688,0.00012316428,0.00011333145,0.0000712547],"domain_scores_gemma":[0.9983006,0.00010366139,0.0004617402,0.00035708377,0.0004584515,0.0003184669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076894846,0.00059399597,0.00036406994,0.004629281,0.00033264613,0.0006934918,0.0010685704,0.00028502184,0.01459109],"category_scores_gemma":[0.0017883145,0.00033405653,0.00018637623,0.006397747,0.00013015936,0.00081881834,0.001380995,0.00039918456,0.007169571],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027814734,0.00024216012,0.5433025,0.0005087826,0.00021033919,0.00029318486,0.000520229,0.0015518874,0.007140792,0.0025965064,0.29830194,0.14505361],"study_design_scores_gemma":[0.000049873135,0.000035535064,0.79558694,0.0000473947,0.000031961143,0.00036695055,0.00021690238,0.0010637719,0.0011228505,0.0005883958,0.20087041,0.000019077117],"about_ca_topic_score_codex":0.02020976,"about_ca_topic_score_gemma":0.012639407,"teacher_disagreement_score":0.02020976,"about_ca_system_score_codex":0.000550317,"about_ca_system_score_gemma":0.0007720396,"threshold_uncertainty_score":0.04881209},"labels":[],"label_agreement":null},{"id":"W2087427291","doi":"10.1086/322244","title":"The Crab Nebula’s Moving Wisps in Radio","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Crab Nebula; Physics; Pulsar; Crab Pulsar; Astrophysics; Astronomy; Heliosphere; Shock (circulatory); Bow shock (aerodynamics); Similarity (geometry); Shock wave; Solar wind; Plasma; Image (mathematics)","score_opus":0.011003309746828257,"score_gpt":0.30426380871250347,"score_spread":0.2932604989656752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087427291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897904,0.000507879,0.0007959463,0.0000804149,0.000022415332,0.000007514127,0.00022903486,0.00007121336,0.008495248],"genre_scores_gemma":[0.99714917,0.00019953203,0.0011213658,0.000056055727,0.00002634892,0.0000053018794,0.00046210707,0.000020627396,0.0009594949],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995863,0.0000028387612,0.0000013768953,0.000010942181,0.000010962956,0.000015140412],"domain_scores_gemma":[0.99983954,0.000016265552,0.00007104678,0.000024979658,0.00002501518,0.000023097253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006173685,0.000108773835,0.000115085815,0.00074342935,0.00021600563,0.0005458832,0.00018277761,0.00020652996,0.0007808045],"category_scores_gemma":[0.00030656706,0.0001645522,0.00012433925,0.000508296,0.00022813116,0.00018417367,0.00033216825,0.0003112039,0.00024184976],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010602531,0.0002234896,0.48573402,0.00030581394,0.0001991805,0.008892032,0.0040033553,0.00585094,0.30550805,0.0049721436,0.009694576,0.17355613],"study_design_scores_gemma":[0.000011839355,0.00003894516,0.9863841,0.000021340225,0.000022222643,0.0013614596,0.0002103485,0.0007358448,0.003311128,0.00024247266,0.0076443763,0.000015920294],"about_ca_topic_score_codex":0.0021783183,"about_ca_topic_score_gemma":0.0035237065,"teacher_disagreement_score":0.0021783183,"about_ca_system_score_codex":0.00019718916,"about_ca_system_score_gemma":0.00005769075,"threshold_uncertainty_score":0.0043312907},"labels":[],"label_agreement":null},{"id":"W2087448197","doi":"10.1088/0004-637x/713/2/1059","title":"LIFETIME OF THE EMBEDDED PHASE OF LOW-MASS STAR FORMATION AND THE ENVELOPE DEPLETION RATES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Star formation; Accretion (finance); Stars; Young stellar object; Gravitational collapse; Phase (matter); Stellar evolution; Exponent; Stellar mass; Protostar","score_opus":0.007018314994117635,"score_gpt":0.24616381595132708,"score_spread":0.23914550095720943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087448197","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981488,0.00006405794,0.0009442191,0.00002744393,0.0000023396742,0.000002815245,0.00012474906,0.00001798976,0.0006674869],"genre_scores_gemma":[0.99950266,0.000026961627,0.00021380241,0.00000389331,0.0000012905148,0.000002831833,0.00013870683,0.0000058364185,0.00010388563],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999418,0.0000074203795,0.000003861239,0.000020915626,0.000008040747,0.000018019911],"domain_scores_gemma":[0.9991322,0.000358041,0.0002171468,0.000076963755,0.00007792313,0.0001377957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044694508,0.00018162493,0.00018655775,0.00027996372,0.00026474195,0.00052668434,0.00044077914,0.00032384592,0.0008561507],"category_scores_gemma":[0.00319754,0.00016325286,0.0003046978,0.0002315175,0.00036317145,0.0005665748,0.00029500943,0.00031896023,0.00012750737],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037469997,0.00012119186,0.37604615,0.000059233986,0.00010251547,0.00029126476,0.000315466,0.57897943,0.02067492,0.011039484,0.00052896776,0.011466691],"study_design_scores_gemma":[0.00003094524,0.00009328136,0.12084051,0.000014491118,0.000029703548,0.00012147448,0.00008229728,0.87199086,0.0037226977,0.002566225,0.00048407444,0.000023432365],"about_ca_topic_score_codex":0.005019473,"about_ca_topic_score_gemma":0.0024573863,"teacher_disagreement_score":0.005019473,"about_ca_system_score_codex":0.0007015119,"about_ca_system_score_gemma":0.00042217533,"threshold_uncertainty_score":0.009980559},"labels":[],"label_agreement":null},{"id":"W2087457606","doi":"10.1086/503824","title":"High‐Mass Star Formation. II. The Mass Function of Submillimeter Clumps in M17","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; James Clerk Maxwell Telescope; Astrophysics; Initial mass function; Power law; Star formation; Stellar mass; Mass distribution; Mass ratio; Stars; Astronomy; Galaxy; Statistics","score_opus":0.007220066357735912,"score_gpt":0.2013330827281874,"score_spread":0.19411301637045147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087457606","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993449,0.000083991865,0.00025118777,0.00000975368,0.0000012165461,0.0000018300076,0.00007700936,0.000010584612,0.00021961117],"genre_scores_gemma":[0.9991398,0.000034154607,0.0004078844,0.0000074331824,0.000002955825,0.0000035903718,0.00024669655,0.00001004178,0.000147383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991786,0.0000081374355,0.000004468551,0.000023705232,0.00001664901,0.000029150564],"domain_scores_gemma":[0.9994299,0.00007750486,0.00024930274,0.00005522102,0.00007858563,0.000109528715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025296648,0.00031005603,0.00021482115,0.000870581,0.00031343143,0.0005956491,0.00041369136,0.00021202683,0.00058255094],"category_scores_gemma":[0.0006723503,0.0002410245,0.00029816845,0.0004986982,0.0003306337,0.00025548146,0.0005004179,0.00023952466,0.0003399069],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006161185,0.00001135125,0.9754165,0.000018612489,0.000030839037,0.00017187811,0.0002568586,0.00074416277,0.017603694,0.00021919675,0.00013175425,0.0053336383],"study_design_scores_gemma":[0.000007398574,0.00003635536,0.99300086,0.000007779326,0.000011114808,0.00027227675,0.000110065885,0.0026851539,0.0030216468,0.00020562838,0.0006363055,0.000005509843],"about_ca_topic_score_codex":0.0036003087,"about_ca_topic_score_gemma":0.005541788,"teacher_disagreement_score":0.0036003087,"about_ca_system_score_codex":0.0005734657,"about_ca_system_score_gemma":0.00013404204,"threshold_uncertainty_score":0.0071586967},"labels":[],"label_agreement":null},{"id":"W2087485601","doi":"10.1086/587446","title":"<i>MOST</i>Space‐based Photometry of the Transiting Exoplanet System HD 209458: Transit Timing to Search for Additional Planets","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Saint Mary's University; St. Mary's University; University of British Columbia","funders":"","keywords":"Exoplanet; Physics; Planet; Transit (satellite); Photometry (optics); Spitzer Space Telescope; Planetary system; Astrophysics; Astronomy; Stars; Radial velocity; Hot Jupiter","score_opus":0.025287883682717477,"score_gpt":0.23699735950337547,"score_spread":0.211709475820658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087485601","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9787441,0.00052840705,0.0020072977,0.00012821423,0.000038114562,0.000028129576,0.01034155,0.00017812941,0.008005999],"genre_scores_gemma":[0.98620075,0.00018928108,0.005062298,0.000094858624,0.000062267616,0.000022140166,0.0074343677,0.00003098749,0.00090301293],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988306,0.000011713847,0.00001268007,0.00003526763,0.00003159266,0.000025782938],"domain_scores_gemma":[0.9995716,0.00004640103,0.0001863812,0.00007385463,0.000060952185,0.000060695682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020903093,0.00022794266,0.0001456634,0.0014524292,0.00034772966,0.000429913,0.00022305643,0.00017150906,0.0017961714],"category_scores_gemma":[0.00038747874,0.00007351776,0.00014370534,0.0008316122,0.00011859556,0.00020650298,0.0004108599,0.00016638509,0.00059855636],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002627442,0.00013931516,0.84584963,0.00016308125,0.00009945692,0.00044400673,0.00033206586,0.0004566888,0.09451392,0.0005546714,0.00594141,0.051243078],"study_design_scores_gemma":[0.000005615903,0.00007609807,0.979681,0.000010601986,0.000025831627,0.000568382,0.00005075794,0.0004053456,0.011158258,0.00011387279,0.007895603,0.000008483482],"about_ca_topic_score_codex":0.002671589,"about_ca_topic_score_gemma":0.005887626,"teacher_disagreement_score":0.002671589,"about_ca_system_score_codex":0.00018098322,"about_ca_system_score_gemma":0.00014122984,"threshold_uncertainty_score":0.0060088634},"labels":[],"label_agreement":null},{"id":"W2087491108","doi":"10.1086/429714","title":"The Broadband Spectrum and Infrared Variability of the Magnetar AXP 1E 1048.1−5937","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Magnetar; Astrophysics; Pulsar; Physics; Infrared; Spectral energy distribution; Flux (metallurgy); Astronomy; Photometry (optics); Context (archaeology); Geology; Chemistry; Stars","score_opus":0.0056376759218082625,"score_gpt":0.2634827046274068,"score_spread":0.25784502870559856,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087491108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99887115,0.000113505674,0.000092583316,0.000016045817,0.0000026087973,9.0989346e-7,0.00011931695,0.000011189186,0.0007725408],"genre_scores_gemma":[0.9991365,0.00008049568,0.00017619203,0.000010824623,0.000012912649,0.0000015418136,0.00038910803,0.000003250637,0.00018922017],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995494,0.0000031076438,0.0000024471956,0.000014787627,0.000011375064,0.000013364338],"domain_scores_gemma":[0.9998461,0.000022970984,0.00007021765,0.0000119857705,0.000017399721,0.000031287735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009871574,0.000182817,0.00012946999,0.00085786264,0.00018228247,0.00025831632,0.00017792487,0.00015376958,0.00066681096],"category_scores_gemma":[0.000296714,0.000070128764,0.00007322683,0.00045635854,0.00015982671,0.00022995574,0.00021513086,0.0001818861,0.00020293839],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003253161,0.00014248188,0.75470424,0.00008342356,0.00008338984,0.0012302096,0.00057190063,0.0013349705,0.19549626,0.0011086795,0.0010846383,0.04383444],"study_design_scores_gemma":[0.0000045457336,0.000050553546,0.99700004,0.0000044496683,0.000014899882,0.00043547328,0.000030711,0.00041920514,0.0012809682,0.000106208645,0.000649456,0.0000036630854],"about_ca_topic_score_codex":0.0011630883,"about_ca_topic_score_gemma":0.002188544,"teacher_disagreement_score":0.0011630883,"about_ca_system_score_codex":0.00020102813,"about_ca_system_score_gemma":0.00003388212,"threshold_uncertainty_score":0.0023126006},"labels":[],"label_agreement":null},{"id":"W2087495064","doi":"10.1086/432526","title":"Discovery of Three Wide‐Orbit Binary Pulsars: Implications for Binary Evolution and Equivalence Principles","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Pulsar; White dwarf; Astrophysics; Millisecond pulsar; Astronomy; Binary number; Binary pulsar; Theoretical physics; Orbital elements; Stars","score_opus":0.030021036807925533,"score_gpt":0.33016505141697855,"score_spread":0.30014401460905304,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087495064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960288,0.00038789609,0.0020780845,0.00013348242,0.000011123477,0.0000049497066,0.000028763969,0.000012088545,0.0013147785],"genre_scores_gemma":[0.99911064,0.00010889629,0.0006154833,0.00003271291,0.00001182557,0.0000030218205,0.00004355854,0.0000015838335,0.00007230699],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999724,0.000037751295,0.00002949738,0.00008432178,0.000076789765,0.000047675847],"domain_scores_gemma":[0.9981744,0.0005303354,0.00078455376,0.0002700865,0.00008931718,0.00015127349],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007603945,0.00014161228,0.00025373485,0.0005458663,0.00086315285,0.0016267983,0.000363692,0.0006053218,0.0006213404],"category_scores_gemma":[0.00270904,0.00017682386,0.00014583851,0.00064613676,0.0012598525,0.0007662139,0.0016074077,0.00069655816,0.00014073862],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043484694,0.0001078303,0.82638305,0.000100870624,0.00006776701,0.0015118644,0.002259688,0.0010630515,0.05057484,0.025178457,0.00030092383,0.092016734],"study_design_scores_gemma":[0.000080170365,0.0005361477,0.8935656,0.00004675654,0.000101063495,0.008728008,0.0012837282,0.0033117621,0.02908575,0.052963227,0.010229402,0.00006842989],"about_ca_topic_score_codex":0.00027758756,"about_ca_topic_score_gemma":0.00025572418,"teacher_disagreement_score":0.0016267983,"about_ca_system_score_codex":0.0002763038,"about_ca_system_score_gemma":0.00015702756,"threshold_uncertainty_score":0.004021406},"labels":[],"label_agreement":null},{"id":"W2087522489","doi":"10.1086/308610","title":"A Chemical Model of the Neutral Envelope of the Planetary Nebula NGC 7027","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Planetary nebula; Physics; Nebula; Astrophysics; Extinction (optical mineralogy); Circumstellar envelope; Astrochemistry; Envelope (radar); Ultraviolet; Asymptotic giant branch; Interstellar medium; Astronomy; Stars; Galaxy","score_opus":0.009100415361550207,"score_gpt":0.2006966319913907,"score_spread":0.1915962166298405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087522489","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8419273,0.0008269481,0.122404285,0.0005587415,0.000052934847,0.00009804619,0.0010088496,0.00028683522,0.032836236],"genre_scores_gemma":[0.9757455,0.00079856854,0.013274932,0.00010159711,0.000032923504,0.00013970098,0.00058871106,0.00004714114,0.009270943],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999409,0.000009827546,0.0000026362115,0.000017193062,0.000016582508,0.000012939768],"domain_scores_gemma":[0.9999198,0.000012677803,0.000015526859,0.000006993887,0.000025513042,0.000019577185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001513327,0.0003822409,0.0002541295,0.0003952007,0.00047947565,0.0007625271,0.0012630954,0.0006113516,0.0017670358],"category_scores_gemma":[0.0002934103,0.00026020553,0.00047756472,0.00027432884,0.0006691827,0.00083985756,0.00040545338,0.00027371905,0.0005824782],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005554257,0.000044342363,0.0053212894,0.000058334037,0.0000289342,0.0003522654,0.00022089822,0.8785762,0.016043698,0.093452975,0.00067849737,0.0051669218],"study_design_scores_gemma":[0.00005640483,0.00007860186,0.0032238106,0.0000090494905,0.000022605751,0.00018178919,0.00008198468,0.96825534,0.00094788027,0.022815574,0.0042992337,0.00002763319],"about_ca_topic_score_codex":0.020237666,"about_ca_topic_score_gemma":0.007765652,"teacher_disagreement_score":0.020237666,"about_ca_system_score_codex":0.0013326609,"about_ca_system_score_gemma":0.0011363697,"threshold_uncertainty_score":0.04023969},"labels":[],"label_agreement":null},{"id":"W2087603551","doi":"10.1086/498393","title":"Oscillations in the Massive Wolf-Rayet Star WR 123 with the <i>M</i> <i>O</i> <i>S</i> <i>T</i> Satellite","year":2005,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto; St. Mary's University; University of British Columbia; Saint Mary's University; Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Wolf–Rayet star; Stellar rotation; Light curve; Astronomy; Variable star; Stars; Rotation period","score_opus":0.009364506424839512,"score_gpt":0.21477084125557205,"score_spread":0.20540633483073253,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087603551","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99961984,0.000016612381,0.000037868907,0.0000042549905,7.032344e-7,0.0000014835513,0.00007040847,0.000004153673,0.00024460236],"genre_scores_gemma":[0.9993266,0.000016183221,0.00020533847,0.000003765772,0.0000026353084,0.000002136015,0.0002499516,0.0000034347113,0.00019006449],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999572,0.0000033183146,0.0000025767165,0.0000129284945,0.0000126589475,0.00001127338],"domain_scores_gemma":[0.9998523,0.000008288508,0.00006470798,0.000011622986,0.000021467487,0.00004154075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000084057974,0.00015336572,0.00014376167,0.00035034673,0.00022978039,0.00027606156,0.00018943436,0.00020865437,0.00037957937],"category_scores_gemma":[0.00021432032,0.00008027212,0.00011395351,0.0003177456,0.00013099257,0.00010464082,0.00022677575,0.00021608372,0.00013556136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038492033,0.00017478492,0.7678157,0.000036369172,0.00009252813,0.0008805639,0.00049696874,0.0012087934,0.21492256,0.000172261,0.0004674865,0.013347031],"study_design_scores_gemma":[0.0000051959923,0.00007034204,0.9955531,0.0000022740735,0.000011381563,0.0001875364,0.00008333496,0.0007580159,0.002982028,0.000022397708,0.00032046737,0.0000040057425],"about_ca_topic_score_codex":0.007005185,"about_ca_topic_score_gemma":0.01318962,"teacher_disagreement_score":0.007005185,"about_ca_system_score_codex":0.00023958336,"about_ca_system_score_gemma":0.00007671599,"threshold_uncertainty_score":0.013928831},"labels":[],"label_agreement":null},{"id":"W2087608172","doi":"10.1086/374597","title":"Radiative Torques on Interstellar Grains. III. Dynamics with Thermal Relaxation","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Radiative transfer; Physics; Thermal; Thermal fluctuations; Torque; Angular momentum; Polarization (electrochemistry); Rotation (mathematics); Thermal radiation; Astrophysics; Mechanics; Computational physics; Classical mechanics; Condensed matter physics; Optics; Chemistry; Meteorology; Thermodynamics","score_opus":0.006162050752752082,"score_gpt":0.21333558490449878,"score_spread":0.2071735341517467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087608172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.73374456,0.005166312,0.19832976,0.0013846827,0.0005876904,0.00020576289,0.0002305233,0.00048829225,0.059862424],"genre_scores_gemma":[0.9878818,0.0006985592,0.0037008377,0.00010030462,0.00008269921,0.00004280361,0.00006647292,0.00008712622,0.007339444],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984765,0.00001724869,0.000007637938,0.000032910903,0.000036018577,0.000058580736],"domain_scores_gemma":[0.9997352,0.00006197783,0.0000751127,0.000056011846,0.00003646144,0.000035289257],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025519126,0.00045021684,0.00046852475,0.00035416867,0.00063488225,0.0009972436,0.00088598725,0.0005292141,0.0034627193],"category_scores_gemma":[0.0010802257,0.00036611807,0.0008016252,0.00030338153,0.0014505674,0.0017529856,0.00090419553,0.00074076146,0.0003379351],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022838883,0.0001464363,0.0069626765,0.0003733734,0.000110631896,0.0011948821,0.00078873534,0.40243444,0.07623896,0.4856641,0.0020212787,0.023836028],"study_design_scores_gemma":[0.00008977376,0.00012656122,0.0082911365,0.000029125185,0.000036177018,0.00028662613,0.00025216507,0.8992391,0.010706785,0.07543121,0.005459679,0.000051630082],"about_ca_topic_score_codex":0.0038959072,"about_ca_topic_score_gemma":0.0018384309,"teacher_disagreement_score":0.0038959072,"about_ca_system_score_codex":0.00097099773,"about_ca_system_score_gemma":0.00036249866,"threshold_uncertainty_score":0.011583984},"labels":[],"label_agreement":null},{"id":"W2087667589","doi":"10.1088/0004-637x/763/1/13","title":"OHMIC HEATING SUSPENDS, NOT REVERSES, THE COOLING CONTRACTION OF HOT JUPITERS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Hot Jupiter; Planet; RADIUS; Joule heating; Radiative cooling; Ohmic contact; Thermal","score_opus":0.0165745670639879,"score_gpt":0.24147049810328328,"score_spread":0.22489593103929537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087667589","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992793,0.00005560505,0.00015622555,0.000011336504,8.8737045e-7,0.0000010738842,0.000015249594,0.000007764746,0.00047262447],"genre_scores_gemma":[0.99978155,0.000025395018,0.00006841677,0.000004103162,0.000002388709,0.000001384513,0.000022484324,0.0000036135323,0.00009075141],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995124,0.000008863601,0.0000020185835,0.0000158951,0.0000059455383,0.000016024456],"domain_scores_gemma":[0.9996445,0.00009938534,0.00013851422,0.000046717636,0.00002225311,0.000048654972],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014689376,0.00016007868,0.00015514324,0.00029035012,0.00028512868,0.00035093707,0.0002999147,0.0002321138,0.0006131664],"category_scores_gemma":[0.0011054145,0.00012246188,0.00018134028,0.00016218523,0.0005031272,0.0004055355,0.00032057843,0.00022599845,0.00011491112],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007405089,0.0001486355,0.5100194,0.0001431464,0.0001763418,0.0022532754,0.0015860093,0.05502796,0.39772263,0.008013476,0.00092446635,0.023244157],"study_design_scores_gemma":[0.00003402422,0.00039447597,0.867784,0.00001971839,0.00007125966,0.00069918233,0.00057907205,0.09548844,0.029824084,0.0024180468,0.0026537604,0.000033947206],"about_ca_topic_score_codex":0.0015833564,"about_ca_topic_score_gemma":0.0010637029,"teacher_disagreement_score":0.0015833564,"about_ca_system_score_codex":0.00030580515,"about_ca_system_score_gemma":0.00007388971,"threshold_uncertainty_score":0.0031482577},"labels":[],"label_agreement":null},{"id":"W2087736624","doi":"10.1086/498610","title":"Aluminum‐Magnesium and Oxygen Isotope Study of Relict Ca‐Al‐rich Inclusions in Chondrules","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Chondrule; Chondrite; Carbonaceous chondrite; Geology; Melilite; Geochemistry; Radiogenic nuclide; Olivine; Formation and evolution of the Solar System; Meteorite; Isotopes of oxygen; Astrobiology; Mineralogy; Physics; Paleontology","score_opus":0.006165755154159469,"score_gpt":0.21866933333157806,"score_spread":0.2125035781774186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087736624","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989618,0.00017641306,0.00014371486,0.0000035915918,0.0000012236814,0.000003988099,0.0001190778,0.000008102218,0.0005821251],"genre_scores_gemma":[0.99848986,0.00008426669,0.00032653776,0.0000062069303,0.0000015469099,0.000003064851,0.00039032157,0.0000075022613,0.0006905507],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993455,0.0000020704622,0.0000046856885,0.000021739486,0.000021065047,0.000015846657],"domain_scores_gemma":[0.9998957,0.000008389117,0.00002113915,0.000009730192,0.00004077154,0.000024323912],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000052853702,0.00019183164,0.00020399143,0.00060895516,0.00029702703,0.00037906878,0.00041019186,0.00025660585,0.00039496098],"category_scores_gemma":[0.00013787532,0.00016626803,0.00018778525,0.00031911017,0.00025593102,0.00016731274,0.00019059479,0.00018585344,0.00018694076],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021671638,0.0000194817,0.027815115,0.000027918171,0.000023296363,0.0003557728,0.0001323878,0.000089856214,0.9693868,0.000064707856,0.000016677508,0.0018511976],"study_design_scores_gemma":[0.00004274776,0.00027293767,0.69190955,0.000014606981,0.000061549385,0.00141845,0.00054515875,0.0032243067,0.2986694,0.00011517102,0.0037064287,0.000019768504],"about_ca_topic_score_codex":0.01165417,"about_ca_topic_score_gemma":0.010444224,"teacher_disagreement_score":0.01165417,"about_ca_system_score_codex":0.0003056198,"about_ca_system_score_gemma":0.00016389765,"threshold_uncertainty_score":0.023172677},"labels":[],"label_agreement":null},{"id":"W2087762119","doi":"10.1088/0004-637x/763/2/121","title":"INTRAGROUP AND GALAXY-LINKED DIFFUSE X-RAY EMISSION IN HICKSON COMPACT GROUPS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Astrophysics; Physics; Galaxy group; Galaxy; Galaxy cluster; Luminosity; Brightest cluster galaxy; Astronomy; Peculiar galaxy; Galaxy groups and clusters; Star formation; Cluster (spacecraft); Type-cD galaxy; Lenticular galaxy","score_opus":0.006965602916975027,"score_gpt":0.2074665155650611,"score_spread":0.20050091264808606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087762119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999696,0.000035344998,0.000028661821,0.0000037059665,3.9888474e-7,0.0000021075223,0.000036061265,0.0000015279751,0.00019628386],"genre_scores_gemma":[0.9996724,0.000024478824,0.000058187707,0.000005770249,0.0000019880133,0.000002223662,0.000114298615,0.0000017743396,0.000118917626],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985945,0.000011678835,0.00001001781,0.00005079726,0.0000254039,0.000042668347],"domain_scores_gemma":[0.99931073,0.00006471618,0.00034934795,0.000053104373,0.000049745224,0.0001722762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017814132,0.00019518555,0.00019590413,0.0014211161,0.00026769482,0.00056762615,0.00021904969,0.00017705887,0.0009277977],"category_scores_gemma":[0.0006674458,0.00013975197,0.00013357174,0.00051170937,0.00043831274,0.00039149314,0.00083616487,0.00020636639,0.00017095459],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011889892,0.000024576411,0.9891081,0.000009231592,0.000021967506,0.00009679272,0.0006311723,0.00005163204,0.007206421,0.0000948861,0.00004247719,0.0025939306],"study_design_scores_gemma":[0.0000017951965,0.000024523215,0.9993291,0.0000023476916,0.000004840849,0.0001272292,0.00018762416,0.00004768784,0.00017840619,0.000030096257,0.00006495381,0.0000014477345],"about_ca_topic_score_codex":0.0036349932,"about_ca_topic_score_gemma":0.005529034,"teacher_disagreement_score":0.0036349932,"about_ca_system_score_codex":0.0002410946,"about_ca_system_score_gemma":0.00008873299,"threshold_uncertainty_score":0.007227659},"labels":[],"label_agreement":null},{"id":"W2087780703","doi":"10.1088/0004-637x/764/1/106","title":"ASSEMBLY OF PROTOPLANETARY DISKS AND INCLINATIONS OF CIRCUMBINARY PLANETS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Circumbinary planet; Planet; Binary number; Accretion (finance); Protoplanetary disk; Binary star; Orbit (dynamics); Binary system; Planetary system","score_opus":0.009818377779101795,"score_gpt":0.23420521637089403,"score_spread":0.22438683859179223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087780703","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9869943,0.0008748992,0.0048861015,0.000024668781,0.0000067370306,0.000007027458,0.0001643702,0.00005876101,0.0069831028],"genre_scores_gemma":[0.99788046,0.00016657409,0.0012890963,0.0000032170644,0.0000022143267,0.0000027293574,0.00013220294,0.00001174949,0.00051178347],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992573,0.000009555193,0.0000041732637,0.000019363431,0.000028200187,0.000012963286],"domain_scores_gemma":[0.99977595,0.0000323803,0.00010563473,0.000027026335,0.000029219036,0.000029842879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000975335,0.00014771362,0.00010203271,0.00051079004,0.00021796238,0.00057707,0.00017975355,0.00014383928,0.0009515692],"category_scores_gemma":[0.00076273317,0.00020757076,0.00009314433,0.0003524205,0.00015387504,0.00027382452,0.00023118396,0.0001165918,0.00026257656],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002455474,0.00006118415,0.7996619,0.00012669757,0.000066363486,0.00051060907,0.000608857,0.030351615,0.11139465,0.0089450525,0.00062725204,0.04740029],"study_design_scores_gemma":[0.0000074752093,0.00003399278,0.9381906,0.000016610436,0.000024629113,0.0004363444,0.00017715248,0.046144165,0.009939884,0.0016472659,0.0033701528,0.000011791173],"about_ca_topic_score_codex":0.0028400496,"about_ca_topic_score_gemma":0.0031264175,"teacher_disagreement_score":0.0028400496,"about_ca_system_score_codex":0.00033533477,"about_ca_system_score_gemma":0.00012762171,"threshold_uncertainty_score":0.0056470037},"labels":[],"label_agreement":null},{"id":"W2087877919","doi":"10.1086/521922","title":"Stellar Evolution in NGC 6791: Mass Loss on the Red Giant Branch and the Formation of Low‐Mass White Dwarfs","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Horizontal branch; White dwarf; Red-giant branch; Astronomy; Red giant; Open cluster; Stellar evolution; Asymptotic giant branch; Galaxy; Stellar population; Red clump; Giant star; Stars; Globular cluster; Metallicity; Star formation","score_opus":0.007026384098129912,"score_gpt":0.20607046031729095,"score_spread":0.19904407621916104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087877919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99931467,0.00010338501,0.0000597518,0.0000058730507,7.665992e-7,0.000001241953,0.00005796095,0.000006185243,0.00045029598],"genre_scores_gemma":[0.9993581,0.000060438644,0.000100409816,0.000007577159,0.0000020658179,0.0000013972546,0.00025339506,0.000004020777,0.0002126635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990845,0.000006553947,0.000005626632,0.00002195108,0.000026005428,0.00003146939],"domain_scores_gemma":[0.9998016,0.000019854877,0.000078867095,0.000018100738,0.000032382424,0.00004918987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110930705,0.00028548064,0.00021295455,0.0006232347,0.00047215272,0.00044200878,0.00025875162,0.00029867887,0.00050282344],"category_scores_gemma":[0.00020845533,0.00008811526,0.00013016704,0.000651281,0.00031106747,0.00020420081,0.00037832776,0.00020368939,0.00034642662],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101818914,0.00004169937,0.9268315,0.000032953903,0.00004038205,0.00071148167,0.00080081436,0.0008238355,0.06254565,0.00029566648,0.00018365248,0.0075906105],"study_design_scores_gemma":[0.0000019854015,0.000036814115,0.9974026,0.000002395299,0.000010191478,0.00037728908,0.00015894,0.00025232485,0.0012076969,0.000048970396,0.00049663853,0.000004099931],"about_ca_topic_score_codex":0.016077865,"about_ca_topic_score_gemma":0.025385879,"teacher_disagreement_score":0.016077865,"about_ca_system_score_codex":0.0004140052,"about_ca_system_score_gemma":0.00015216718,"threshold_uncertainty_score":0.031968594},"labels":[],"label_agreement":null},{"id":"W2087892528","doi":"10.1086/506008","title":"Detailed Atmosphere Modeling for the Neutron Star 1E1207.4−5209: Evidence of Oxygen/Neon Atmosphere","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Atmosphere (unit); Neon; Oxygen; Physics; Atomic physics; Thermodynamics; Argon","score_opus":0.020973459136144255,"score_gpt":0.30919476566218684,"score_spread":0.2882213065260426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087892528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98629063,0.00012691121,0.009887749,0.00010576892,0.000008781225,0.000018819357,0.00052729406,0.00018535728,0.002848568],"genre_scores_gemma":[0.9932587,0.00012001111,0.0054717963,0.000024823104,0.000010185788,0.000016496848,0.0005241197,0.000047992016,0.00052582874],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995625,0.000009440135,0.0000027141393,0.000010376753,0.000011338267,0.0000098718565],"domain_scores_gemma":[0.99991393,0.000022784707,0.000021784572,0.000010201162,0.000013341887,0.000017882146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013054106,0.00034657907,0.00031031866,0.00029192507,0.00031744794,0.00036079518,0.0005819272,0.0004390334,0.00069285993],"category_scores_gemma":[0.0003221179,0.00018625187,0.00052474416,0.00018075161,0.00017438515,0.00036099402,0.000340044,0.00025351287,0.000098206474],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000070133254,0.00006238316,0.025524035,0.000030274661,0.000053498094,0.00016081243,0.00007681094,0.9574788,0.009451372,0.0026517634,0.00023320012,0.004206882],"study_design_scores_gemma":[0.000022315351,0.000039857856,0.0063100723,0.0000025269069,0.000013958518,0.000032354248,0.000021793241,0.9917326,0.0006807243,0.0006182595,0.00051686144,0.000008691716],"about_ca_topic_score_codex":0.012556846,"about_ca_topic_score_gemma":0.009315138,"teacher_disagreement_score":0.012556846,"about_ca_system_score_codex":0.00049757166,"about_ca_system_score_gemma":0.00043968298,"threshold_uncertainty_score":0.024967551},"labels":[],"label_agreement":null},{"id":"W2087961809","doi":"10.1088/0004-637x/786/2/120","title":"DISK-LOSS AND DISK-RENEWAL PHASES IN CLASSICAL Be STARS. II. CONTRASTING WITH STABLE AND VARIABLE DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Balmer series; Polarization (electrochemistry); Stars; Cosmology; Position angle; Variable star; Line-of-sight; Light curve","score_opus":0.008608042710751255,"score_gpt":0.22349471461319428,"score_spread":0.21488667190244304,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2087961809","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983505,0.00022964805,0.00030780016,0.000012852361,0.0000012434116,0.0000052834084,0.000060244154,0.000004614797,0.0010279668],"genre_scores_gemma":[0.9993024,0.00008545903,0.00020345482,0.000009362528,0.0000046817304,0.0000043485475,0.00014364092,0.0000016751464,0.00024488193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983406,0.000013881761,0.000014779045,0.0000597694,0.00003027825,0.000047261114],"domain_scores_gemma":[0.9991788,0.00013915682,0.00034636576,0.000083644365,0.00009478564,0.00015713231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019172175,0.00013039177,0.00017226709,0.001127711,0.0004543915,0.00081904617,0.00032390832,0.00031646315,0.000824668],"category_scores_gemma":[0.0012274846,0.000108709115,0.0001347898,0.00063506415,0.000764708,0.00072112423,0.0007516153,0.00029583072,0.00021678246],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005262183,0.000100186204,0.94990295,0.00005941013,0.000028337647,0.00039716085,0.0007375502,0.0005431339,0.028186567,0.0014877378,0.00008546381,0.017945357],"study_design_scores_gemma":[0.0000042520123,0.000087323344,0.99482286,0.0000044696185,0.000006733923,0.00045955804,0.00043583315,0.00074662914,0.0020955433,0.0008421857,0.00048969896,0.000004938121],"about_ca_topic_score_codex":0.0015253955,"about_ca_topic_score_gemma":0.00240954,"teacher_disagreement_score":0.0015253955,"about_ca_system_score_codex":0.00038457717,"about_ca_system_score_gemma":0.00016578693,"threshold_uncertainty_score":0.003033042},"labels":[],"label_agreement":null},{"id":"W2088089730","doi":"10.1086/345400","title":"New Mass Estimators For Tracer Populations","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Globular cluster; Estimator; TRACER; Physics; Galaxy; Dark matter; Halo; Astrophysics; Population; Monte Carlo method; Boltzmann equation; Cluster (spacecraft); Stars; Statistics; Mathematics; Nuclear physics; Computer science","score_opus":0.022183899853945293,"score_gpt":0.2624266277143865,"score_spread":0.24024272786044124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088089730","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0075791427,0.00057315984,0.9889985,0.00014766221,0.00015022159,0.000065723856,0.00030079024,0.0005654034,0.0016194261],"genre_scores_gemma":[0.18943302,0.0013643075,0.79533273,0.000519571,0.00092005957,0.0007269762,0.0025220464,0.00089193764,0.008289338],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99677026,0.0009324917,0.000195836,0.0010491927,0.00079020945,0.00026211902],"domain_scores_gemma":[0.98510695,0.007682116,0.0018015943,0.0026465033,0.002178729,0.00058420585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0067768595,0.001091069,0.0012722815,0.004928741,0.0010124337,0.0039070905,0.0040645534,0.0023860591,0.005020633],"category_scores_gemma":[0.054367337,0.00084313424,0.001067792,0.002578649,0.0019202634,0.0092337495,0.0039115003,0.00337069,0.0020705755],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018545656,0.00015149695,0.047094416,0.00022124033,0.00028920293,0.0002417711,0.00066289044,0.10404602,0.005847299,0.59070873,0.008250749,0.24230078],"study_design_scores_gemma":[0.000077692646,0.00010558917,0.0051198313,0.00015362518,0.000088016815,0.0005684563,0.00012411343,0.55629283,0.0049010143,0.39595821,0.036470905,0.00013978078],"about_ca_topic_score_codex":0.0019918045,"about_ca_topic_score_gemma":0.00143327,"teacher_disagreement_score":0.0067768595,"about_ca_system_score_codex":0.0016798722,"about_ca_system_score_gemma":0.0011474272,"threshold_uncertainty_score":0.035839856},"labels":[],"label_agreement":null},{"id":"W2088104909","doi":"10.1088/0004-637x/777/2/126","title":"LUMINOUS INFRARED GALAXIES WITH THE SUBMILLIMETER ARRAY. IV.<sup>12</sup>CO<i>J</i>= 6-5 OBSERVATIONS OF VV 114","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Submillimeter Array; Galaxy; Astrophysics; Nucleus; Millimeter; Line (geometry); Milky Way; Infrared; Luminous infrared galaxy; Radiative transfer; Astronomy; Star formation; Optics","score_opus":0.014366490314234752,"score_gpt":0.2123861101764535,"score_spread":0.19801961986221875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088104909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7722224,0.0013219093,0.060712855,0.00075325975,0.00026642263,0.00040632216,0.057793856,0.01225325,0.09426969],"genre_scores_gemma":[0.86871207,0.00039799584,0.06535751,0.0003847008,0.0002355358,0.0002720578,0.050376266,0.0005306047,0.01373318],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981016,0.000025878633,0.000009337415,0.000052099294,0.00006818268,0.000034416884],"domain_scores_gemma":[0.999491,0.00007130623,0.000148628,0.00014767869,0.000059723996,0.00008171964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026473563,0.00027969904,0.00021405586,0.0007188212,0.00024106106,0.00060753484,0.0007656775,0.00030935125,0.011064529],"category_scores_gemma":[0.0005714709,0.00024441569,0.00050325086,0.00072542176,0.0001456234,0.0003298205,0.00050388643,0.0004691406,0.003465715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005729076,0.00017123242,0.71981055,0.00022442189,0.00028951923,0.0002152963,0.0003362871,0.005403201,0.06254072,0.003844752,0.037820112,0.16877097],"study_design_scores_gemma":[0.000050546958,0.00011465567,0.9411428,0.000029443878,0.00008381391,0.00020524436,0.00006718196,0.008552208,0.006981137,0.0014015797,0.0413514,0.000020003716],"about_ca_topic_score_codex":0.003935981,"about_ca_topic_score_gemma":0.008620457,"teacher_disagreement_score":0.011064529,"about_ca_system_score_codex":0.00024559043,"about_ca_system_score_gemma":0.00014326329,"threshold_uncertainty_score":0.037014544},"labels":[],"label_agreement":null},{"id":"W2088182181","doi":"10.1088/0004-637x/692/1/149","title":"ON THE AGE OF THE WIDEST VERY LOW MASS BINARY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Binary number; Observatory; Sky; Binary star; Low Mass; Proper motion; Brown dwarf; Spectroscopy","score_opus":0.009080709821599406,"score_gpt":0.20829134484027362,"score_spread":0.1992106350186742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088182181","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99427503,0.0013345152,0.00024662667,0.00018670927,0.00003172134,0.000003308246,0.000089938905,0.000008126539,0.0038238766],"genre_scores_gemma":[0.9989693,0.00020039539,0.00008199393,0.000045765853,0.00001958071,0.000001699759,0.00013260152,0.0000026323619,0.00054614036],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989045,0.000010445989,0.000006700023,0.000030870757,0.000019805559,0.000041754032],"domain_scores_gemma":[0.99940526,0.0001142112,0.00018581018,0.00003987041,0.00012799444,0.00012689656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048630522,0.00010369964,0.00027350592,0.00096948916,0.0013787524,0.0015631478,0.0002888385,0.000596074,0.0014691848],"category_scores_gemma":[0.0016982307,0.00012625696,0.000089830406,0.0004084064,0.00036510744,0.00080131507,0.0007915062,0.00051663484,0.0005220568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007452557,0.00009560725,0.9093411,0.000060025166,0.00003209394,0.001532942,0.0010799994,0.00044840077,0.035902258,0.0077256025,0.00092674344,0.04210997],"study_design_scores_gemma":[0.000015245821,0.00013164403,0.97139364,0.00004043254,0.000029638684,0.003795858,0.00071765034,0.0011852891,0.006951269,0.003816592,0.011900218,0.000022565044],"about_ca_topic_score_codex":0.0024566795,"about_ca_topic_score_gemma":0.002470184,"teacher_disagreement_score":0.0024566795,"about_ca_system_score_codex":0.0007288223,"about_ca_system_score_gemma":0.00024563982,"threshold_uncertainty_score":0.0052879453},"labels":[],"label_agreement":null},{"id":"W2088233588","doi":"10.1086/529488","title":"The Most Dark‐Matter–dominated Galaxies: Predicted Gamma‐Ray Signals from the Faintest Milky Way Dwarfs","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Galaxy; Dwarf galaxy; Dark matter; Dwarf galaxy problem; Dwarf spheroidal galaxy; Luminosity; Local Group","score_opus":0.007672965696073037,"score_gpt":0.20463514549226497,"score_spread":0.19696217979619193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088233588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953973,0.00004586239,0.00021032576,0.000011293665,4.115813e-7,7.052162e-7,0.000043445663,0.0000120943305,0.00013624158],"genre_scores_gemma":[0.99963546,0.000022805336,0.00014434132,0.0000045736156,0.0000019223303,7.7272864e-7,0.00014741479,0.000002415384,0.00004022056],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999193,0.000013463385,0.0000051194506,0.00002468039,0.000013312447,0.000024023382],"domain_scores_gemma":[0.9991032,0.00020366699,0.00031671405,0.000106024636,0.00007084809,0.00019958949],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048745645,0.00036865097,0.00036059192,0.00091431785,0.00024764243,0.000961473,0.00041447056,0.00031351243,0.00040463073],"category_scores_gemma":[0.0012247505,0.00025199543,0.0003508528,0.00037219655,0.00038817732,0.0002823214,0.0005031377,0.00021471345,0.00013861446],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000957099,0.000012703556,0.9869676,0.000011513201,0.000034927867,0.00009791392,0.00014685058,0.0027736062,0.007079555,0.0003398622,0.0000525075,0.0023873043],"study_design_scores_gemma":[0.00002258559,0.00004298419,0.9842025,0.0000074024824,0.00004181699,0.00016671424,0.00010597304,0.0104995845,0.0037190798,0.00075154274,0.0004270836,0.000012749095],"about_ca_topic_score_codex":0.004312718,"about_ca_topic_score_gemma":0.00535355,"teacher_disagreement_score":0.004312718,"about_ca_system_score_codex":0.00052367634,"about_ca_system_score_gemma":0.00016952759,"threshold_uncertainty_score":0.008575261},"labels":[],"label_agreement":null},{"id":"W2088264501","doi":"10.1086/368280","title":"Experimental Transition Rate of the Green Coronal Line of Fe<scp>xiv</scp>","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atomic and Molecular Physics","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Atomic physics; Electron beam ion trap; Line (geometry); Coronal plane; Ion; Dipole; Plasma; Ground state; Electron; Astrophysics; Cathode ray; Nuclear physics; Quantum mechanics","score_opus":0.008513482649736432,"score_gpt":0.22707272947541943,"score_spread":0.218559246825683,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088264501","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905372,0.00025171763,0.0050620106,0.000042771982,0.000012879445,0.000019861627,0.0007996069,0.00014023509,0.0031336013],"genre_scores_gemma":[0.9973611,0.00009564899,0.0014599251,0.000014137682,0.0000033533695,0.000016826742,0.00061042735,0.00001647185,0.00042215496],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9997185,0.000041415024,0.000009189995,0.00012313008,0.000056355755,0.000051443323],"domain_scores_gemma":[0.99938095,0.00028808406,0.00012523704,0.0000656248,0.00009291359,0.00004717905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060336164,0.0002644483,0.00014656175,0.0004416144,0.000407728,0.00034444773,0.000538677,0.00045665333,0.002433972],"category_scores_gemma":[0.00098011,0.00016905302,0.00014040634,0.00030075997,0.0004136135,0.00036534053,0.00019654662,0.00044626603,0.00030110197],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012104185,0.00015637823,0.036212612,0.00015626253,0.00007897279,0.00020718762,0.00032868102,0.0014317026,0.94590306,0.002316617,0.000729007,0.011269195],"study_design_scores_gemma":[0.0000527176,0.00043414245,0.07225338,0.000012991987,0.000043210213,0.00029456845,0.00007957866,0.0055592544,0.91852987,0.00033846032,0.0023764542,0.000025322302],"about_ca_topic_score_codex":0.0017756105,"about_ca_topic_score_gemma":0.0016080339,"teacher_disagreement_score":0.002433972,"about_ca_system_score_codex":0.00047366894,"about_ca_system_score_gemma":0.00013487632,"threshold_uncertainty_score":0.008142471},"labels":[],"label_agreement":null},{"id":"W2088563093","doi":"10.1088/0004-637x/793/2/102","title":"ERASING THE VARIABLE: EMPIRICAL FOREGROUND DISCOVERY FOR GLOBAL 21 cm SPECTRUM EXPERIMENTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Polarization (electrochemistry); Faraday effect; Synchrotron radiation; Amplitude; Synchrotron; Sky; Magnetic monopole; Calibration; Spectral leakage; Cosmic background radiation","score_opus":0.01740883406785351,"score_gpt":0.27785863115290477,"score_spread":0.2604497970850513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088563093","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26024556,0.0009264606,0.73465395,0.0006545229,0.000024370627,0.000037785947,0.0003286327,0.00073247566,0.0023962639],"genre_scores_gemma":[0.7936757,0.0004642022,0.20375822,0.00027549692,0.00007736446,0.00009012325,0.0006035815,0.0002908443,0.0007643834],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989409,0.0005000131,0.00003584056,0.00027344222,0.00018256603,0.000067278255],"domain_scores_gemma":[0.984312,0.010835203,0.0015307447,0.0027194559,0.0003178452,0.00028475892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0062352996,0.00066530623,0.00078273285,0.000693692,0.0005762266,0.0012686084,0.0010435927,0.0008329842,0.001054994],"category_scores_gemma":[0.021249278,0.00042894774,0.00037403195,0.0007344445,0.0018351994,0.0020328618,0.0020960146,0.0014607655,0.00018570677],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014888513,0.00043750403,0.15405287,0.0004840987,0.00075917615,0.00040667132,0.0008338845,0.14819442,0.10285776,0.15890756,0.0028914106,0.42868575],"study_design_scores_gemma":[0.00013351477,0.00036272453,0.10203522,0.00012467754,0.00022813102,0.00041834038,0.00029602557,0.6290946,0.041232646,0.21431172,0.011640324,0.000122022946],"about_ca_topic_score_codex":0.00063816726,"about_ca_topic_score_gemma":0.000963883,"teacher_disagreement_score":0.0062352996,"about_ca_system_score_codex":0.0005891742,"about_ca_system_score_gemma":0.00047970403,"threshold_uncertainty_score":0.032975793},"labels":[],"label_agreement":null},{"id":"W2088616187","doi":"10.1086/499332","title":"Discovery of Multiple Coaxial Rings in the Quadrupolar Planetary Nebula NGC 6881","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Planetary nebula; Asymptotic giant branch; Torus; Astrophysics; Bipolar nebula; Nebula; Bipolar outflow; Astronomy; Protoplanetary nebula; Stars; Geometry; Star formation","score_opus":0.009598065147263921,"score_gpt":0.21657272120775542,"score_spread":0.2069746560604915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088616187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99667203,0.0007362617,0.0005361084,0.000053068605,0.000015017073,0.000007239785,0.00009585155,0.000042321688,0.0018421119],"genre_scores_gemma":[0.9980367,0.00023538595,0.0011752547,0.000036881,0.000023242306,0.000005174494,0.00014824342,0.0000051488087,0.00033412583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984324,0.0000134565325,0.000007888493,0.00006136214,0.000034817218,0.000039211776],"domain_scores_gemma":[0.9993993,0.00006847624,0.00022673978,0.00014752621,0.000049569004,0.000108355125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016475772,0.00017873784,0.00015217182,0.000694275,0.00055779127,0.0007599809,0.0003167925,0.00043834298,0.0007535277],"category_scores_gemma":[0.0004976713,0.00025351022,0.00011309259,0.00030283767,0.00036883954,0.00047737427,0.0006977797,0.00028337605,0.00038562293],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053328753,0.00010983348,0.48768732,0.00021038644,0.00016127381,0.017188663,0.002184834,0.00084530166,0.41031274,0.0029963816,0.0022637069,0.07550621],"study_design_scores_gemma":[0.000057525118,0.00038657035,0.8976155,0.00006341416,0.00012011787,0.037625846,0.0006372289,0.0018736594,0.031604845,0.0019647386,0.027954716,0.00009591932],"about_ca_topic_score_codex":0.00049945386,"about_ca_topic_score_gemma":0.0010231151,"teacher_disagreement_score":0.0007599809,"about_ca_system_score_codex":0.00013195338,"about_ca_system_score_gemma":0.000071208204,"threshold_uncertainty_score":0.0025207996},"labels":[],"label_agreement":null},{"id":"W2088634301","doi":"10.1086/428750","title":"<i>FUSE</i>Observations of DB White Dwarfs","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Université de Montréal","funders":"","keywords":"Physics; White dwarf; Astrophysics; Stars; Spectral line; Carbon star; Astronomy; Carbon fibers; Stellar classification; Ultraviolet; Stellar atmosphere; Optics","score_opus":0.016761800799191973,"score_gpt":0.22667105534843945,"score_spread":0.20990925454924747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088634301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99224746,0.00059359847,0.00067419105,0.000029419522,0.0000039520523,0.0000049272253,0.0031238846,0.00008883867,0.0032338433],"genre_scores_gemma":[0.9922955,0.0002734391,0.0012320924,0.000040540817,0.000013801134,0.0000033471445,0.0054259705,0.000016160477,0.000699056],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998896,0.0000045211614,0.000007639775,0.000021073341,0.00004585098,0.000031217267],"domain_scores_gemma":[0.9997905,0.000017759536,0.000065947126,0.00002385164,0.000037915022,0.000064057276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012960933,0.00021580761,0.00015938675,0.0024657946,0.00044748606,0.00034888036,0.00013758916,0.00018429733,0.00062496145],"category_scores_gemma":[0.00017957797,0.00010499025,0.00019019848,0.00092773495,0.0001322311,0.00023932925,0.00029811187,0.00013415751,0.0002517291],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003533947,0.000087334454,0.76453954,0.00012619328,0.00014751154,0.00079789857,0.0011654494,0.0010653506,0.18052964,0.00055735244,0.0022736322,0.04835669],"study_design_scores_gemma":[0.0000026159603,0.000039701856,0.9853914,0.0000068456015,0.00003339497,0.0006202507,0.00012888918,0.0002721528,0.009027603,0.00015075183,0.004317037,0.000009395402],"about_ca_topic_score_codex":0.008321907,"about_ca_topic_score_gemma":0.018688269,"teacher_disagreement_score":0.008321907,"about_ca_system_score_codex":0.00033462356,"about_ca_system_score_gemma":0.000117460884,"threshold_uncertainty_score":0.016546965},"labels":[],"label_agreement":null},{"id":"W2088671121","doi":"10.1088/0004-637x/760/1/78","title":"AN EMPIRICAL MEASURE OF THE RATE OF WHITE DWARF COOLING IN 47 TUCANAE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Université de Montréal; University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"Globular cluster; White dwarf; Astrophysics; Physics; Sequence (biology); Cluster (spacecraft); Measure (data warehouse); White (mutation); Field (mathematics); Astronomy; Stars; Mathematics; Biology; Computer science; Genetics","score_opus":0.019527693639252695,"score_gpt":0.259758102088257,"score_spread":0.2402304084490043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088671121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966666,0.00009124936,0.0016057002,0.000015527317,0.0000013114269,0.0000044722683,0.00023406667,0.000047326732,0.00133364],"genre_scores_gemma":[0.9985226,0.000045525125,0.0008157922,0.000003953302,0.0000021377678,0.00000516638,0.0004266105,0.000011730709,0.00016654909],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983716,0.00001582533,0.0000078648145,0.00005475489,0.000044531585,0.000039848517],"domain_scores_gemma":[0.99859065,0.00036725125,0.00047249786,0.00017198993,0.00032497323,0.0000725963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040015366,0.0001458833,0.0001329562,0.0014393972,0.00035145704,0.00042649705,0.00044700367,0.00026873534,0.000765266],"category_scores_gemma":[0.0034683298,0.000120288714,0.00012794462,0.00096280314,0.00038247564,0.00044117027,0.00025407985,0.0002381036,0.0001783575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003883462,0.000009196784,0.9778642,0.000014433938,0.000038529543,0.000038203318,0.00021425633,0.0054286392,0.0063992282,0.0004910952,0.00015542,0.009308101],"study_design_scores_gemma":[0.0000014407725,0.000008968585,0.9890754,0.0000040438767,0.000006190876,0.000108607834,0.00007450347,0.007501792,0.002479755,0.00020632311,0.00052694743,0.0000060568495],"about_ca_topic_score_codex":0.03682403,"about_ca_topic_score_gemma":0.041499726,"teacher_disagreement_score":0.03682403,"about_ca_system_score_codex":0.00090039603,"about_ca_system_score_gemma":0.0003486531,"threshold_uncertainty_score":0.07321936},"labels":[],"label_agreement":null},{"id":"W2088753075","doi":"10.1086/515392","title":"The Unusual Binary Pulsar PSR J1744−3922: Radio Flux Variability, Near‐Infrared Observation, and Evolution","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Toronto; McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Magnetar; Binary pulsar; White dwarf; Neutron star; Millisecond pulsar; Pulsar planet; Astronomy; Accretion (finance); X-ray pulsar; Orbital period; Stars","score_opus":0.012111795877667399,"score_gpt":0.29689762441942397,"score_spread":0.28478582854175655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088753075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99926466,0.00010172196,0.000118199234,0.000017139197,0.0000034994198,0.0000046015416,0.00010600162,0.0000110284445,0.00037322412],"genre_scores_gemma":[0.9989022,0.000054639037,0.00037153834,0.000019423303,0.000017864733,0.0000093727385,0.00041914402,0.000005875275,0.00019996864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999928,0.000008330113,0.0000045360366,0.000021387941,0.000021486483,0.000016297146],"domain_scores_gemma":[0.9998035,0.000021355076,0.000090899346,0.000013957985,0.000014261721,0.000055969806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013230187,0.0002636794,0.00023372631,0.0008779345,0.0004834134,0.00037744053,0.00021386796,0.0002929505,0.0006193382],"category_scores_gemma":[0.00033587168,0.000096615324,0.000080101294,0.0007474041,0.00031285643,0.00019684294,0.0003924503,0.00024778885,0.0001966064],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037329397,0.00014724213,0.81089336,0.00006874818,0.00008620207,0.0046287496,0.0004033005,0.000381728,0.16282241,0.00032915786,0.000822482,0.019043485],"study_design_scores_gemma":[0.000014400963,0.00013624375,0.9914886,0.000002477297,0.00001436282,0.004207232,0.000106164734,0.00033396133,0.0025184962,0.00012834556,0.0010408149,0.000008952],"about_ca_topic_score_codex":0.0010717686,"about_ca_topic_score_gemma":0.0012362584,"teacher_disagreement_score":0.0010717686,"about_ca_system_score_codex":0.00021522996,"about_ca_system_score_gemma":0.00010264421,"threshold_uncertainty_score":0.0021310449},"labels":[],"label_agreement":null},{"id":"W2088827965","doi":"10.1088/0004-637x/761/1/71","title":"BARYONS MATTER: WHY LUMINOUS SATELLITE GALAXIES HAVE REDUCED CENTRAL MASSES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":333,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Reionization; Satellite galaxy; Galaxy; Star formation; Supernova; Astronomy; Accretion (finance); Milky Way; Stars; Dark matter; Dwarf galaxy; Redshift","score_opus":0.009189665007260416,"score_gpt":0.21430624090686834,"score_spread":0.2051165758996079,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088827965","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975719,0.00007186507,0.0009762367,0.00020842318,0.000005234369,0.0000028736185,0.00006759983,0.000055811495,0.0010400498],"genre_scores_gemma":[0.9994211,0.000022701463,0.00035383838,0.000024132902,0.0000018782458,0.0000016958295,0.000026965341,0.000013006042,0.00013462716],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991906,0.000019214083,0.0000040911013,0.000023609102,0.000013255864,0.00002079633],"domain_scores_gemma":[0.99956554,0.00011420043,0.00011358654,0.00005958622,0.00003897703,0.00010811177],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023673772,0.00021456282,0.00024468076,0.00020627078,0.00023787444,0.0008827132,0.00056685705,0.00050470384,0.0013883817],"category_scores_gemma":[0.0025163635,0.0001720299,0.00018613008,0.0001996073,0.00049869675,0.00041610777,0.00039491185,0.00023795315,0.00016906801],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091303064,0.00016862298,0.57918304,0.00033257663,0.0002381767,0.0011388517,0.001712331,0.27376276,0.085334085,0.033650998,0.002130553,0.021435024],"study_design_scores_gemma":[0.000437081,0.00018122543,0.24535914,0.00006843758,0.00016354502,0.000402936,0.0010209426,0.69968534,0.02726165,0.022218896,0.0031483285,0.000052527685],"about_ca_topic_score_codex":0.0070984247,"about_ca_topic_score_gemma":0.007698681,"teacher_disagreement_score":0.0070984247,"about_ca_system_score_codex":0.0004255717,"about_ca_system_score_gemma":0.0002680787,"threshold_uncertainty_score":0.014114261},"labels":[],"label_agreement":null},{"id":"W2088832460","doi":"10.1086/430632","title":"Two Pulsar Wind Nebulae:<i>Chandra/XMM‐Newton</i>Imaging of GeV J1417−6100","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Aeronautics and Space Administration","keywords":"Pulsar; Physics; Astrophysics; Acis; Nebula; Pulsar wind nebula; Astronomy; Point source; Pulsar planet; Binary pulsar; Millisecond pulsar; Stars; Optics","score_opus":0.00938245010604639,"score_gpt":0.3113270892763535,"score_spread":0.3019446391703071,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088832460","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974546,0.00015148449,0.00028150744,0.000028441467,0.0000068494924,0.00001615212,0.00030503538,0.00003415304,0.0017217349],"genre_scores_gemma":[0.99259174,0.0001616041,0.0041124304,0.000080304664,0.000021496577,0.000030809784,0.0021520217,0.000032691016,0.0008168651],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999019,0.000003932495,0.0000053732583,0.000021599575,0.000033963337,0.00003326307],"domain_scores_gemma":[0.9997142,0.000019842617,0.00008465065,0.00003499487,0.000033086882,0.00011318924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013593429,0.00020366648,0.0002817218,0.0010490842,0.00046345143,0.0005472609,0.00034532562,0.0003213523,0.00096733565],"category_scores_gemma":[0.00027248773,0.0002398963,0.00018033192,0.00059496996,0.00022183776,0.00026529076,0.0007056157,0.0003670099,0.00025842394],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009957964,0.0004243892,0.40062818,0.00017162316,0.00016678144,0.0057164505,0.0009775758,0.00079115934,0.54910177,0.001168226,0.001842806,0.038015217],"study_design_scores_gemma":[0.000055694425,0.00015222604,0.9738539,0.000016473921,0.00003398855,0.0032330672,0.000108861095,0.0008099477,0.016549008,0.00020400676,0.0049612094,0.000021536673],"about_ca_topic_score_codex":0.001738544,"about_ca_topic_score_gemma":0.0057731587,"teacher_disagreement_score":0.001738544,"about_ca_system_score_codex":0.0002100685,"about_ca_system_score_gemma":0.00021695117,"threshold_uncertainty_score":0.003456831},"labels":[],"label_agreement":null},{"id":"W2088969683","doi":"10.1088/0004-637x/802/2/75","title":"THE ROLE OF TURBULENCE AND MAGNETIC FIELDS IN SIMULATED FILAMENTARY STRUCTURE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; McMaster University; Herzberg Institute of Astrophysics","funders":"","keywords":"Protein filament; Substructure; Magnetic field; Magnetohydrodynamics; Turbulence; Magnetohydrodynamic drive; Isothermal process; Solar prominence; Relaxation (psychology)","score_opus":0.005338814823444769,"score_gpt":0.21464857088073874,"score_spread":0.20930975605729396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088969683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99605185,0.000045121426,0.0019861856,0.00007485496,0.000007236178,0.00001349728,0.00015262053,0.00008899297,0.0015796165],"genre_scores_gemma":[0.9985952,0.000022897326,0.001074261,0.000013675774,0.0000023553155,0.000009711162,0.00012299654,0.000021272956,0.00013755808],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998802,0.000030073708,0.000006963276,0.000015992451,0.000024122353,0.00004273606],"domain_scores_gemma":[0.9990816,0.0004585987,0.00015381648,0.00007405831,0.00009382933,0.00013808705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041302506,0.0004293214,0.00035769504,0.00050623645,0.0006127426,0.00076207495,0.0006929358,0.0006482129,0.00072612416],"category_scores_gemma":[0.0024124999,0.00026973724,0.00041040345,0.0005572559,0.0006756545,0.000456282,0.00038414757,0.00046800898,0.000074456046],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012899922,0.000078116274,0.021534376,0.000019374802,0.000044734858,0.00011368692,0.00010893271,0.9719579,0.0031556068,0.0013284099,0.0001582921,0.0013716556],"study_design_scores_gemma":[0.000029575824,0.00004122861,0.0038950169,0.000005696169,0.000009792094,0.000016140615,0.000038878134,0.9944748,0.0009968588,0.00035181665,0.00013049328,0.00000964383],"about_ca_topic_score_codex":0.021665351,"about_ca_topic_score_gemma":0.010593743,"teacher_disagreement_score":0.021665351,"about_ca_system_score_codex":0.0012054823,"about_ca_system_score_gemma":0.000676289,"threshold_uncertainty_score":0.04307854},"labels":[],"label_agreement":null},{"id":"W2088972242","doi":"10.1088/0004-637x/777/1/66","title":"SHOCK-ENHANCED C<sup>+</sup>EMISSION AND THE DETECTION OF H<sub>2</sub>O FROM THE STEPHAN'S QUINTET GROUP-WIDE SHOCK USING<i>HERSCHEL</i>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Protein filament; Line (geometry); Spectral line; Galaxy; Shock (circulatory); Excitation; Cosmic ray; Emission spectrum; Shock wave; Atomic physics; Astronomy; Chemistry; Geometry","score_opus":0.007362856347278335,"score_gpt":0.20866185179673563,"score_spread":0.20129899544945729,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2088972242","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9852874,0.000098245546,0.0011149802,0.00017798337,0.000014626256,0.000016225295,0.0011036962,0.00014066839,0.012045961],"genre_scores_gemma":[0.99493885,0.00003262818,0.0015684568,0.000103494254,0.000015255841,0.00000856425,0.0009595623,0.000026480822,0.0023467615],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994004,0.0000015693709,0.0000011115885,0.000016913522,0.00002446948,0.000016019541],"domain_scores_gemma":[0.9998411,0.000015553886,0.00005456588,0.000020623163,0.000020481357,0.00004758104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059359772,0.00017380313,0.000064756445,0.0003557551,0.0002815824,0.00022481193,0.00036618017,0.00030670298,0.005479355],"category_scores_gemma":[0.00019806235,0.00012229651,0.000106244624,0.00038049978,0.00029930257,0.00016996493,0.000368161,0.000267555,0.0005207418],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003542782,0.00005778316,0.27450347,0.00010610429,0.000064705186,0.0037614799,0.00045749274,0.0004989319,0.68896323,0.0017124416,0.004158188,0.025361875],"study_design_scores_gemma":[0.000008092922,0.000060136532,0.9465879,0.000005759725,0.000016444585,0.0019774362,0.00012960029,0.0009085175,0.04179132,0.00029039296,0.008212986,0.0000113558835],"about_ca_topic_score_codex":0.0029941811,"about_ca_topic_score_gemma":0.01145225,"teacher_disagreement_score":0.005479355,"about_ca_system_score_codex":0.00028968818,"about_ca_system_score_gemma":0.00014396606,"threshold_uncertainty_score":0.018330276},"labels":[],"label_agreement":null},{"id":"W2089081255","doi":"10.1086/308275","title":"Isochrones and Luminosity Functions for Old White Dwarfs","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"White dwarf; Globular cluster; Astrophysics; Physics; Luminosity; Luminosity function; Massive compact halo object; Cluster (spacecraft); Sirius; Halo; Open cluster; Opacity; White (mutation); Blue dwarf; Astronomy; Stars; Galaxy; Computer science; Biology","score_opus":0.009874490148591293,"score_gpt":0.21675269646609105,"score_spread":0.20687820631749976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089081255","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47277677,0.00036550045,0.50080687,0.00007364795,0.00007111907,0.000063981446,0.0027544228,0.0040919124,0.01899577],"genre_scores_gemma":[0.8674448,0.00031028723,0.120411575,0.000022890821,0.000024608578,0.000088812725,0.0049783024,0.00084608776,0.0058725653],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99985933,0.000027769984,0.0000094699835,0.000040726572,0.000043660788,0.000019162175],"domain_scores_gemma":[0.9995097,0.00009539487,0.000049972736,0.0001597175,0.00015044563,0.000034791305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005665473,0.0002634364,0.000301143,0.0010552342,0.00035482598,0.0008364612,0.0006823972,0.00024165728,0.0024164715],"category_scores_gemma":[0.0016089564,0.00023129488,0.00057264837,0.00070041703,0.00027016498,0.00053526956,0.0003300734,0.00040302734,0.0011074946],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014492383,0.00007723818,0.11221592,0.00007788852,0.000101310536,0.00012912789,0.00069142785,0.77525413,0.012988859,0.041113947,0.004542147,0.052663025],"study_design_scores_gemma":[0.00003193522,0.00007038668,0.042356763,0.000016078511,0.00007132493,0.00022934581,0.000116893854,0.9156863,0.00926587,0.012701495,0.019389033,0.00006456434],"about_ca_topic_score_codex":0.00847946,"about_ca_topic_score_gemma":0.00744078,"teacher_disagreement_score":0.00847946,"about_ca_system_score_codex":0.0009964444,"about_ca_system_score_gemma":0.00049671443,"threshold_uncertainty_score":0.016860187},"labels":[],"label_agreement":null},{"id":"W2089097543","doi":"10.1088/0004-637x/783/1/58","title":"TRACING THE OUTFLOW OF A<i>z</i>= 0.334 FeLoBAL: NEW CONSTRAINTS FROM LOW-IONIZATION ABSORBERS IN FBQS J1151+3822","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Outflow; Photoionization; Quasar; Absorption (acoustics); RADIUS; Ionization; Luminosity; Hydrogen; Line (geometry)","score_opus":0.009081473878382623,"score_gpt":0.21642442544892448,"score_spread":0.20734295157054186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089097543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981433,0.00012406487,0.00050282635,0.00003613859,0.0000031588122,0.0000037100122,0.00015269834,0.000022524619,0.0010114583],"genre_scores_gemma":[0.9988423,0.00003959948,0.0005657196,0.000020121985,0.000007355394,0.0000022364989,0.0003577281,0.000008969283,0.00015602265],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999144,0.000005381469,0.0000026644675,0.000025530378,0.000012684193,0.000039398958],"domain_scores_gemma":[0.9997178,0.00003415729,0.00008989426,0.00001581964,0.00002365871,0.00011871079],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018967112,0.00026232886,0.00030928315,0.0010453605,0.00049823563,0.00074273965,0.0003594108,0.00044918442,0.0010721183],"category_scores_gemma":[0.00042816316,0.00016329458,0.00019283587,0.0004353842,0.00023637661,0.000427521,0.0007202884,0.00031721743,0.00022931465],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029420006,0.00012693611,0.9068766,0.000056474662,0.000048314276,0.0016288204,0.0011790165,0.0009806318,0.07411496,0.0007888135,0.0006561314,0.01324905],"study_design_scores_gemma":[0.000010842918,0.000049473412,0.9924109,0.000016459675,0.00001727043,0.00030901225,0.00030614465,0.0032666505,0.0017896227,0.00023543974,0.0015772389,0.000010950192],"about_ca_topic_score_codex":0.009092179,"about_ca_topic_score_gemma":0.019291295,"teacher_disagreement_score":0.009092179,"about_ca_system_score_codex":0.0004591332,"about_ca_system_score_gemma":0.00017040467,"threshold_uncertainty_score":0.018078506},"labels":[],"label_agreement":null},{"id":"W2089118837","doi":"10.1086/383516","title":"The Formation of a Realistic Disk Galaxy in Λ‐dominated Cosmologies","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":270,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy formation and evolution; Astronomy; Galaxy; Galaxy merger; Interacting galaxy; Dark matter halo; Bulge; Cold dark matter; Satellite galaxy; Dark matter; Star formation; Angular momentum; Halo","score_opus":0.008059079052636406,"score_gpt":0.22139894720207817,"score_spread":0.21333986814944178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089118837","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99350727,0.00004327498,0.002024919,0.000085708576,0.0000071305085,0.000011915781,0.00015820864,0.000040428684,0.0041211387],"genre_scores_gemma":[0.9972778,0.00004857053,0.0016480469,0.0000264371,0.0000030062577,0.000012677873,0.00014503441,0.000013994342,0.00082450727],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999199,0.000027666347,0.0000029396306,0.000015420936,0.00000914314,0.000024898347],"domain_scores_gemma":[0.999676,0.00010182208,0.000048455862,0.00003759324,0.000038324615,0.00009769095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000290152,0.0002488531,0.0002651178,0.00031475018,0.00044324782,0.00087232766,0.00068468304,0.0007474942,0.0017657678],"category_scores_gemma":[0.001375813,0.00024603854,0.0003091157,0.00035130946,0.00070440397,0.0007154424,0.00075997255,0.0003962753,0.00017008845],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018767334,0.00008610267,0.01857355,0.000025149022,0.00003947737,0.00022825744,0.000170065,0.9675959,0.0016010447,0.0095326705,0.00034061965,0.0016195881],"study_design_scores_gemma":[0.0001292037,0.00012044613,0.005368425,0.000008466741,0.000019746365,0.000050495953,0.00015288456,0.99009246,0.0007569126,0.0024221756,0.00086391397,0.000014882838],"about_ca_topic_score_codex":0.024708282,"about_ca_topic_score_gemma":0.0122807985,"teacher_disagreement_score":0.024708282,"about_ca_system_score_codex":0.0011968423,"about_ca_system_score_gemma":0.0005372572,"threshold_uncertainty_score":0.04912889},"labels":[],"label_agreement":null},{"id":"W2089204210","doi":"10.1086/588650","title":"On the Enhancement of Mass Loss in Cepheids Due to Radial Pulsation","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cepheid variable; Astrophysics; Physics; Instability strip; Astronomy; Stars","score_opus":0.012470210106761782,"score_gpt":0.22249632195912467,"score_spread":0.2100261118523629,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089204210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79422027,0.0018492527,0.18754402,0.00023963641,0.000045521054,0.00007559906,0.00040666934,0.00066271954,0.014956244],"genre_scores_gemma":[0.9802799,0.0006461503,0.017447183,0.000031175026,0.0000473617,0.00003198629,0.00017705263,0.000074381205,0.0012648429],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982053,0.000036143334,0.000009917044,0.000034331282,0.00006777522,0.00003134317],"domain_scores_gemma":[0.99828136,0.0010396269,0.00035819865,0.00015361854,0.00012265024,0.000044515713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008306207,0.00046721916,0.00019074877,0.001333986,0.00021036815,0.00037599073,0.0005987712,0.00018329335,0.0012712332],"category_scores_gemma":[0.0050974963,0.00016652857,0.00032141202,0.00067717646,0.00052583165,0.00054211495,0.0006915452,0.0003686155,0.00051789975],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050940906,0.00010679775,0.34799963,0.00037210848,0.00011148854,0.0022531445,0.0008522129,0.3294084,0.064213656,0.04173655,0.0017735972,0.21066299],"study_design_scores_gemma":[0.00002192874,0.0001722255,0.4271523,0.00006042392,0.00005168568,0.0019372643,0.000087056345,0.527797,0.021973671,0.015981289,0.0047102696,0.000054964425],"about_ca_topic_score_codex":0.0015289227,"about_ca_topic_score_gemma":0.00086319196,"teacher_disagreement_score":0.0015289227,"about_ca_system_score_codex":0.0004265865,"about_ca_system_score_gemma":0.000121184064,"threshold_uncertainty_score":0.0043928027},"labels":[],"label_agreement":null},{"id":"W2089214555","doi":"10.1088/0004-637x/703/2/1308","title":"ROTATION OF THE WARM MOLECULAR GAS SURROUNDING ULTRACOMPACT H II REGIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Star formation; Rotation (mathematics); Line (geometry); Stars; Geometry","score_opus":0.01093210069822283,"score_gpt":0.24962876492490926,"score_spread":0.23869666422668642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089214555","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995408,0.000048445334,0.00015921028,0.0000043056725,5.749257e-7,6.764384e-7,0.000012537986,0.0000066875505,0.00022674269],"genre_scores_gemma":[0.9996649,0.000023484663,0.00022784735,0.0000031581897,0.0000032301468,6.9278764e-7,0.00003714943,0.0000015953814,0.000037890633],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995065,0.0000057909097,0.0000018462038,0.000017744993,0.000008660202,0.00001527335],"domain_scores_gemma":[0.9998011,0.000033890195,0.00010048988,0.000018546369,0.000009436167,0.000036614525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011803991,0.00015140776,0.0001432783,0.0003987713,0.00027659716,0.0003657441,0.00022762167,0.00012933598,0.00043200384],"category_scores_gemma":[0.0002946238,0.00015514751,0.00012467452,0.00022618989,0.00027388378,0.00022820316,0.00030190137,0.00015556083,0.00008967788],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005782213,0.00008897441,0.5334519,0.000052967916,0.0001446655,0.00039815716,0.0007293936,0.005257502,0.44435737,0.0010065641,0.00013119592,0.013803008],"study_design_scores_gemma":[0.000024822226,0.000166692,0.9716572,0.000007642193,0.000044644396,0.00026043368,0.00015647203,0.0073899897,0.019146653,0.00035561842,0.0007784521,0.000011291596],"about_ca_topic_score_codex":0.0012225221,"about_ca_topic_score_gemma":0.0016648569,"teacher_disagreement_score":0.0012225221,"about_ca_system_score_codex":0.00026573325,"about_ca_system_score_gemma":0.00008439797,"threshold_uncertainty_score":0.0024308562},"labels":[],"label_agreement":null},{"id":"W2089243480","doi":"10.1086/590427","title":"Scattered-Light Echoes from the Historical Galactic Supernovae Cassiopeia A and Tycho (SN 1572)","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Cassiopeia A; Supernova; Milky Way; Supernova remnant; Galactic astronomy; Echo (communications protocol); Spectroscopy","score_opus":0.01609835843327738,"score_gpt":0.21713841251661434,"score_spread":0.20104005408333697,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089243480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990577,0.00017144959,0.0001736997,0.000009204315,0.000006718234,0.000002317835,0.00010616712,0.000009413095,0.00046339398],"genre_scores_gemma":[0.99851567,0.0001305646,0.00041212596,0.000011547879,0.000016995698,0.0000026865848,0.0005926218,0.000010464276,0.00030733043],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999157,0.00000489198,0.000004553422,0.00002695973,0.000027323762,0.000020653599],"domain_scores_gemma":[0.9994498,0.00007616315,0.00018043185,0.00010296131,0.0000844571,0.00010626947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015255115,0.0002734577,0.00018645515,0.0010183457,0.00034854678,0.00062743406,0.0003044835,0.0002927163,0.0009254431],"category_scores_gemma":[0.0005653177,0.0001654179,0.00020320695,0.0009234423,0.00033535555,0.00019485697,0.0007637114,0.00031699883,0.00020176801],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082831626,0.00009030848,0.71231997,0.00014903102,0.00029493825,0.00941752,0.0008246959,0.0003461384,0.25772268,0.00041359031,0.0005565519,0.017036352],"study_design_scores_gemma":[0.000023346623,0.00021840318,0.95296174,0.00001769738,0.000108385415,0.011072812,0.00030775912,0.0006391063,0.031122765,0.00017246345,0.0033318806,0.000023653047],"about_ca_topic_score_codex":0.0019869853,"about_ca_topic_score_gemma":0.0037144402,"teacher_disagreement_score":0.0019869853,"about_ca_system_score_codex":0.0001957902,"about_ca_system_score_gemma":0.00010660215,"threshold_uncertainty_score":0.0039508343},"labels":[],"label_agreement":null},{"id":"W2089310227","doi":"10.1086/522574","title":"The Haunted Halos of Andromeda and Triangulum: A Panorama of Galaxy Formation in Action","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":407,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Milky Way; Astronomy; Andromeda; Galaxy; Halo; Dwarf galaxy; Surface brightness; Galactic halo; Stellar density; Andromeda Galaxy; Local Group","score_opus":0.009875076170922979,"score_gpt":0.23504272283555244,"score_spread":0.22516764666462946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089310227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9487474,0.0055832937,0.002004123,0.0002841215,0.000049827915,0.000031298474,0.0014514115,0.00023631222,0.041612223],"genre_scores_gemma":[0.99418086,0.0007524575,0.002077797,0.00006151012,0.000021773616,0.000005371861,0.0009973795,0.000057469333,0.0018453988],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997365,0.00005622889,0.0000061163933,0.0000662064,0.000069145375,0.00006581728],"domain_scores_gemma":[0.999747,0.000025135056,0.000058218193,0.00005415293,0.000024796116,0.000090785405],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002285801,0.00032547925,0.00023399657,0.0013109153,0.0007340302,0.001266292,0.0004200896,0.00020797648,0.003255238],"category_scores_gemma":[0.0005201004,0.00022688755,0.00031501107,0.001271347,0.0006199037,0.0005475672,0.0017106803,0.00028484446,0.00056912977],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052983727,0.000062159685,0.74135774,0.0004426437,0.0005202805,0.0010962738,0.0105758365,0.002859835,0.03478149,0.024222557,0.008371882,0.1751795],"study_design_scores_gemma":[0.00001003749,0.000076211,0.92844063,0.00006688121,0.000068945585,0.0012742976,0.0024202452,0.00091109826,0.0012195492,0.0014264307,0.06405037,0.000035357174],"about_ca_topic_score_codex":0.011656334,"about_ca_topic_score_gemma":0.027967399,"teacher_disagreement_score":0.011656334,"about_ca_system_score_codex":0.00043393398,"about_ca_system_score_gemma":0.0003244071,"threshold_uncertainty_score":0.023176968},"labels":[],"label_agreement":null},{"id":"W2089346948","doi":"10.1086/375151","title":"Simulations of Galaxy Formation in a ΛCDM Universe. III. The Dissipative Formation of an Elliptical Galaxy","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Elliptical galaxy; Lenticular galaxy; Galaxy; Galaxy merger; Surface brightness fluctuation; Satellite galaxy; Interacting galaxy; Galaxy formation and evolution; Astronomy; Accretion (finance)","score_opus":0.010178518070167957,"score_gpt":0.23030611057206968,"score_spread":0.22012759250190173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089346948","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9839342,0.00013630341,0.004545001,0.0003907727,0.000040081155,0.00006338728,0.0014326324,0.0002591352,0.0091984365],"genre_scores_gemma":[0.9891235,0.00011594369,0.0072767753,0.00013468546,0.000018712417,0.000116558214,0.0011746326,0.000056454028,0.001982671],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983954,0.000056929806,0.000006665789,0.000020536894,0.000023997745,0.00005235075],"domain_scores_gemma":[0.9990706,0.00041742105,0.000093520706,0.00006686263,0.00015065601,0.00020095351],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051110564,0.00039034034,0.00056118687,0.0005848252,0.0005758824,0.00076987164,0.0012085445,0.0012463435,0.0033403789],"category_scores_gemma":[0.002291069,0.00033848907,0.0005858774,0.0007459067,0.0006822782,0.000536455,0.00083085307,0.0010159304,0.00031427314],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027606802,0.00016873833,0.018008541,0.000061030154,0.00006573839,0.00020372139,0.00020901882,0.9701147,0.0009755313,0.00667284,0.0010637536,0.0021802955],"study_design_scores_gemma":[0.00010951397,0.00005378689,0.0035384533,0.000010860096,0.000013919807,0.000025645428,0.00009423864,0.9934809,0.0002788056,0.0016082444,0.00077423285,0.000011401697],"about_ca_topic_score_codex":0.03492676,"about_ca_topic_score_gemma":0.016932065,"teacher_disagreement_score":0.03492676,"about_ca_system_score_codex":0.0014129948,"about_ca_system_score_gemma":0.0007930052,"threshold_uncertainty_score":0.06944698},"labels":[],"label_agreement":null},{"id":"W2089369009","doi":"10.1086/381699","title":"The Space Density of Redshift 5.7 Lyα Emitters: First Constraints from a Multislit Windows Search","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Redshift; Astrophysics; Galaxy; Lyman limit; Intergalactic travel; Reionization; Population; Ionization; Spectral line; Emission spectrum; Flux (metallurgy); Sky; Astronomy; Intergalactic medium; Chemistry","score_opus":0.008807491422390738,"score_gpt":0.2165818490290165,"score_spread":0.20777435760662577,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089369009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996657,0.00015429634,0.0014735633,0.00002891847,8.8961133e-7,0.0000060570983,0.0008056911,0.000042489362,0.0008310944],"genre_scores_gemma":[0.9952224,0.000068393114,0.0023736765,0.0000129857835,0.0000051510087,0.000007668037,0.0020582345,0.000012865868,0.00023865465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962497,0.00006398672,0.00003288177,0.00007706304,0.000086784734,0.00011432437],"domain_scores_gemma":[0.9976053,0.00089162,0.00073297875,0.00020305623,0.0001827603,0.00038429737],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089636736,0.00028741363,0.000426893,0.0016944049,0.0004224666,0.0010600418,0.00046512636,0.00031075653,0.0021586623],"category_scores_gemma":[0.0019727526,0.0001844596,0.00041136311,0.00080431,0.00023917231,0.00058360014,0.00087128516,0.00023855467,0.00055108307],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007045872,0.00007660453,0.9440293,0.000061902196,0.00009199191,0.00040713622,0.00035504907,0.0014885828,0.029632252,0.0018833725,0.00064284186,0.020626565],"study_design_scores_gemma":[0.000031876763,0.00012921027,0.9757985,0.000018127012,0.000082541315,0.0006673148,0.0002895309,0.01203347,0.008038794,0.0012828615,0.0016045994,0.000023215334],"about_ca_topic_score_codex":0.003969933,"about_ca_topic_score_gemma":0.0053459583,"teacher_disagreement_score":0.003969933,"about_ca_system_score_codex":0.0002908444,"about_ca_system_score_gemma":0.00025200238,"threshold_uncertainty_score":0.0078936815},"labels":[],"label_agreement":null},{"id":"W2089382722","doi":"10.1088/0004-637x/712/2/1191","title":"CHEMODYNAMICS OF COMPACT STELLAR SYSTEMS IN NGC 5128: HOW SIMILAR ARE GLOBULAR CLUSTERS, ULTRA-COMPACT DWARFS, AND DWARF GALAXIES?","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Waterloo; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Velocity dispersion; Galaxy; Dwarf galaxy; Elliptical galaxy; Photometry (optics); Astronomy; Fundamental plane (elliptical galaxies); Star cluster; Solar mass; Disc galaxy; Stars","score_opus":0.006797971108735725,"score_gpt":0.20644987060389441,"score_spread":0.19965189949515869,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089382722","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99957985,0.00005404411,0.000025099549,0.000011908404,2.9892817e-7,8.5178806e-7,0.0000459546,0.0000025189172,0.0002794587],"genre_scores_gemma":[0.9997671,0.000019864061,0.000045640067,0.0000026562818,6.1656436e-7,8.3937e-7,0.00006722059,5.1024244e-7,0.00009558338],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999522,0.000005578279,0.0000037885022,0.00001775057,0.000007924431,0.000012791283],"domain_scores_gemma":[0.9996586,0.000050201113,0.00015087512,0.000030258043,0.00003047306,0.000079622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010520954,0.00011861253,0.00011822026,0.00071330136,0.00019255256,0.00037890204,0.00018548309,0.00018621795,0.00066667085],"category_scores_gemma":[0.0005939855,0.00008297386,0.000074290016,0.00049812905,0.00035623004,0.00041625695,0.00035706168,0.000110018,0.00017705467],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000062093444,0.000015242112,0.9837583,0.000009392005,0.000010982922,0.00008298954,0.00037269926,0.00034216366,0.01023053,0.0002973694,0.000060202197,0.0047581303],"study_design_scores_gemma":[0.0000013922071,0.000018848232,0.9984819,0.000002145446,0.0000030512188,0.00009248653,0.0002267266,0.0006794018,0.00024468088,0.00013041498,0.00011661328,0.0000022614352],"about_ca_topic_score_codex":0.0120056365,"about_ca_topic_score_gemma":0.019686392,"teacher_disagreement_score":0.0120056365,"about_ca_system_score_codex":0.0005802537,"about_ca_system_score_gemma":0.00011621484,"threshold_uncertainty_score":0.023871481},"labels":[],"label_agreement":null},{"id":"W2089406568","doi":"10.1086/507605","title":"Multiwavelength Variability of the Magnetar 4U 0142+61","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Magnetar; Photometry (optics); Astrophysics; Infrared; Flux (metallurgy); Physics; Astronomy; Materials science; Pulsar; Stars","score_opus":0.006275210829954078,"score_gpt":0.26722553246320885,"score_spread":0.26095032163325477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089406568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999553,0.000071597206,0.000057486977,0.000011892549,0.0000025417326,0.0000016160212,0.000048115195,0.0000036602205,0.00025016372],"genre_scores_gemma":[0.9992574,0.000050286028,0.00019397412,0.0000148660665,0.000010814571,0.0000048071497,0.0003361768,0.0000029849582,0.00012863807],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997286,0.00004511861,0.000023087381,0.00007963448,0.00006881177,0.000054725508],"domain_scores_gemma":[0.99904984,0.00012986493,0.0003406548,0.00015179218,0.00015567217,0.00017225687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005173407,0.000230742,0.0004708556,0.0010076103,0.0006005679,0.0007539748,0.00028212686,0.00034002372,0.00042284533],"category_scores_gemma":[0.0010791596,0.0002489321,0.0001948932,0.00068624667,0.00037909206,0.0003747349,0.001072621,0.0003026974,0.00014943517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001716757,0.00011301572,0.94999224,0.00005464395,0.0002324394,0.0005077563,0.00086381036,0.0008282664,0.029401982,0.00025609456,0.0003104296,0.017267624],"study_design_scores_gemma":[0.000006040735,0.000058697162,0.9979538,0.000006233546,0.00002259684,0.00029257088,0.000117485324,0.00026252586,0.00046068925,0.000060166883,0.00075254956,0.0000065664676],"about_ca_topic_score_codex":0.0013937193,"about_ca_topic_score_gemma":0.003953349,"teacher_disagreement_score":0.0013937193,"about_ca_system_score_codex":0.00018532203,"about_ca_system_score_gemma":0.00014571674,"threshold_uncertainty_score":0.0027712584},"labels":[],"label_agreement":null},{"id":"W2089415780","doi":"10.1088/0004-637x/724/1/572","title":"THE PLERIONIC SUPERNOVA REMNANT G21.5–0.9 POWERED BY PSR J1833–1034: NEW SPECTROSCOPIC AND IMAGING RESULTS REVEALED WITH THE<i>CHANDRA X-RAY OBSERVATORY</i>","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Supernova remnant; Pulsar wind nebula; Halo; Observatory; Pulsar; Luminosity; ROSAT; Spectral index; RADIUS; Astronomy; Supernova; Spectral line; Galaxy","score_opus":0.004780899749806237,"score_gpt":0.20168688226928985,"score_spread":0.1969059825194836,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089415780","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989452,0.00018053055,0.000060007245,0.00001869714,0.0000018890934,0.0000032147188,0.00015924322,0.00001374989,0.0006175228],"genre_scores_gemma":[0.99895763,0.0001321615,0.0001582267,0.0000143838,0.000012900196,0.0000017617072,0.00047888057,0.000006495565,0.00023758691],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993944,0.0000047263097,0.0000046191367,0.000018151502,0.000014289134,0.000018769766],"domain_scores_gemma":[0.9998173,0.000012336788,0.00006351431,0.000022900833,0.00002484487,0.000059176844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016150592,0.00033219677,0.00024597568,0.00075653236,0.00031651655,0.00067070103,0.00024339734,0.00022769111,0.00043690272],"category_scores_gemma":[0.00021375605,0.00015403226,0.0003345196,0.0005575619,0.00030955777,0.00024837285,0.0003657526,0.00021489328,0.0002387317],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073666545,0.00018233208,0.79986066,0.000102212136,0.00021623394,0.008046499,0.0006442748,0.0012028503,0.17293234,0.0006000161,0.00077219954,0.014703748],"study_design_scores_gemma":[0.0000041654007,0.00005660098,0.99482226,0.0000033949643,0.00003051912,0.0013839742,0.00007228552,0.0003569328,0.0023071363,0.000062868654,0.00089323753,0.0000065622385],"about_ca_topic_score_codex":0.0032626418,"about_ca_topic_score_gemma":0.0036665364,"teacher_disagreement_score":0.0032626418,"about_ca_system_score_codex":0.00024834537,"about_ca_system_score_gemma":0.00006935835,"threshold_uncertainty_score":0.00648731},"labels":[],"label_agreement":null},{"id":"W2089608227","doi":"10.1088/0004-637x/767/2/142","title":"HOT ELECTROMAGNETIC OUTFLOWS. I. ACCELERATION AND SPECTRA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Lorentz factor; Photon; Bremsstrahlung; Magnetic field; Magnetohydrodynamics; Lorentz force; Compton scattering; Gamma-ray burst; Radiation","score_opus":0.008134185576393017,"score_gpt":0.2099838471164297,"score_spread":0.2018496615400367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089608227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95326024,0.0018994668,0.029031994,0.00018110186,0.000034468336,0.000023824276,0.00017667313,0.00038844763,0.015003774],"genre_scores_gemma":[0.9974687,0.00018063441,0.001374725,0.00002812298,0.000038506292,0.000004570401,0.000055147728,0.000029226936,0.0008203494],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990726,0.0000185182,0.000003918926,0.000025309448,0.000019195011,0.0000257682],"domain_scores_gemma":[0.9995109,0.00009824544,0.00022646059,0.000050598082,0.000031137337,0.00008267346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022491826,0.00042621355,0.00025196825,0.00066876103,0.00039834826,0.00086656417,0.00035876178,0.00034413673,0.0012563044],"category_scores_gemma":[0.00075716054,0.0002424387,0.00024154464,0.0003812172,0.00081836974,0.0007360009,0.0010945341,0.00047234804,0.00022791006],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013268387,0.00021910436,0.17366719,0.0005523615,0.00017258423,0.0040099053,0.0021242208,0.08497401,0.33146355,0.31719762,0.003289761,0.08100281],"study_design_scores_gemma":[0.00016476389,0.00032685098,0.38039702,0.00010805459,0.000084141364,0.0047445395,0.0005394682,0.27033946,0.053448632,0.27887836,0.010814766,0.00015398629],"about_ca_topic_score_codex":0.00031410242,"about_ca_topic_score_gemma":0.00016181328,"teacher_disagreement_score":0.0012563044,"about_ca_system_score_codex":0.00042482972,"about_ca_system_score_gemma":0.00005569106,"threshold_uncertainty_score":0.004202783},"labels":[],"label_agreement":null},{"id":"W2089981966","doi":"10.1086/512080","title":"Overcoming Migration during Giant Planet Formation","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gas giant; Jovian; Accretion (finance); Giant planet; Planet; Collision; Hot Jupiter; Range (aeronautics)","score_opus":0.008474186092789472,"score_gpt":0.22642460288666774,"score_spread":0.21795041679387828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2089981966","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98306745,0.00035172104,0.010744056,0.00030623082,0.000027528698,0.000008705013,0.000040503906,0.000073911295,0.005379844],"genre_scores_gemma":[0.99854517,0.00007906217,0.00082177954,0.000009637459,0.0000036891752,0.0000032591772,0.0000106430825,0.000005328039,0.00052152755],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987125,0.000027422291,0.0000045216607,0.000022328166,0.000017390736,0.000057060322],"domain_scores_gemma":[0.99938095,0.00018785949,0.0001599234,0.000086931934,0.0000366043,0.00014772595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027515553,0.0002160423,0.00022934156,0.00019094093,0.00054786005,0.0009937042,0.0004346997,0.00057028333,0.0018593541],"category_scores_gemma":[0.0026817329,0.00021908728,0.00027555457,0.00012686447,0.0005638801,0.0014120169,0.002086557,0.00036215896,0.00018388554],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001340818,0.00017138082,0.10322382,0.000334214,0.0001222936,0.002640261,0.0032961085,0.664729,0.05123343,0.1181987,0.002418389,0.0522916],"study_design_scores_gemma":[0.00013221333,0.0007377862,0.04109782,0.00008249054,0.00008860449,0.0018193375,0.0027211136,0.8698443,0.010176291,0.060985733,0.012232581,0.00008178024],"about_ca_topic_score_codex":0.004194395,"about_ca_topic_score_gemma":0.003118167,"teacher_disagreement_score":0.004194395,"about_ca_system_score_codex":0.00050309335,"about_ca_system_score_gemma":0.00066476024,"threshold_uncertainty_score":0.008340001},"labels":[],"label_agreement":null},{"id":"W2090139880","doi":"10.1088/0004-637x/747/2/143","title":"MODELING THE NEAR-UV BAND OF GK STARS. II. NON-LTE MODELS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Saint Mary's University","funders":"","keywords":"Metallicity; Astrophysics; Physics; Opacity; Effective temperature; Stars; Stellar classification; Atmospheric models; Spectral line; Astronomy","score_opus":0.019358970956451334,"score_gpt":0.23095964233162236,"score_spread":0.21160067137517102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090139880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83793664,0.0005563921,0.13450196,0.00037417054,0.000085667525,0.00006462751,0.0035664556,0.0010682314,0.021845846],"genre_scores_gemma":[0.9757951,0.00025758837,0.01648222,0.00013426806,0.00003087199,0.000055016808,0.0016831715,0.00018795939,0.0053739683],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989974,0.00001675431,0.000005782983,0.000031353964,0.000020095356,0.000026101805],"domain_scores_gemma":[0.9998604,0.000032229265,0.000022632501,0.000030711613,0.00003737495,0.000016554233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014323568,0.00040586214,0.000270881,0.00028843535,0.00035578018,0.0007449417,0.0012116659,0.0006505641,0.0017074569],"category_scores_gemma":[0.0006163348,0.00024153222,0.00072039955,0.0004669992,0.00028231333,0.00096864667,0.00048508344,0.0004506613,0.00072832033],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000081253165,0.000064665066,0.046000063,0.0000639551,0.00010684276,0.00013103551,0.000286864,0.91817284,0.0068220533,0.016176386,0.0017639156,0.010330108],"study_design_scores_gemma":[0.000014250914,0.000017475879,0.0076663443,0.000007051472,0.000020151765,0.00007125022,0.0000687297,0.9826074,0.000991839,0.005594612,0.002926627,0.000014212763],"about_ca_topic_score_codex":0.037963424,"about_ca_topic_score_gemma":0.028166905,"teacher_disagreement_score":0.037963424,"about_ca_system_score_codex":0.00078166137,"about_ca_system_score_gemma":0.00047533205,"threshold_uncertainty_score":0.07548487},"labels":[],"label_agreement":null},{"id":"W2090170291","doi":"10.1088/0004-637x/698/2/l94","title":"EVIDENCE FOR LONG-TERM GAMMA-RAY AND X-RAY VARIABILITY FROM THE UNIDENTIFIED TeV SOURCE HESS J0632+057","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Term (time); X-ray; Gamma ray; Physics; Biology; Astrophysics; Astronomy; Nuclear physics","score_opus":0.02325838289413349,"score_gpt":0.26204612477972555,"score_spread":0.23878774188559207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090170291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989011,0.00010166005,0.00007747856,0.000018416376,0.0000044721546,0.000002322689,0.00016553035,0.000008406243,0.00072053605],"genre_scores_gemma":[0.9986463,0.00005389738,0.00014703722,0.000025006639,0.000010467522,0.0000038901226,0.0008382728,0.0000052437063,0.0002697363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998692,0.000009840309,0.000011009153,0.00003258602,0.0000465228,0.000030874875],"domain_scores_gemma":[0.99929285,0.00010532794,0.0002358279,0.00009394829,0.00012326315,0.00014874572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018954258,0.0001599313,0.00030009745,0.00062937394,0.00034552978,0.0006871478,0.00036127958,0.00043337033,0.0012363265],"category_scores_gemma":[0.00050608354,0.00018422178,0.00015720779,0.00068630616,0.00028131704,0.00026431395,0.00046976685,0.00029704007,0.0004571102],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032200283,0.00010128598,0.8946261,0.00007969711,0.00008821026,0.0022261962,0.0004251406,0.00045947757,0.09132533,0.00050397083,0.00073488755,0.009107809],"study_design_scores_gemma":[0.0000128242245,0.00009430014,0.99489367,0.000008863609,0.000018914641,0.0012236966,0.00014339204,0.00042743972,0.001992229,0.00010725239,0.0010675634,0.000009965033],"about_ca_topic_score_codex":0.0018819162,"about_ca_topic_score_gemma":0.0036635308,"teacher_disagreement_score":0.0018819162,"about_ca_system_score_codex":0.0002907812,"about_ca_system_score_gemma":0.00014466264,"threshold_uncertainty_score":0.0041359067},"labels":[],"label_agreement":null},{"id":"W2090208590","doi":"10.1086/588091","title":"Inclination‐Independent Galaxy Classification","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Sky; Lenticular galaxy; Galaxy formation and evolution; Interacting galaxy; Galaxy merger; Peculiar galaxy; Dwarf galaxy","score_opus":0.016280765973494767,"score_gpt":0.23035423759445356,"score_spread":0.2140734716209588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090208590","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.32739097,0.0014646129,0.5757997,0.00031918232,0.00036854387,0.0007896305,0.017804338,0.012774188,0.06328877],"genre_scores_gemma":[0.6256878,0.00045762362,0.33999038,0.00016597274,0.00017036167,0.0004946919,0.021792606,0.0006958957,0.0105447145],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9985239,0.00014622037,0.0001296496,0.00038693636,0.0006223662,0.00019092168],"domain_scores_gemma":[0.99649006,0.00026777212,0.00062911457,0.0010269425,0.0013677898,0.00021831406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009553737,0.00062304025,0.0006104451,0.007082636,0.000716474,0.0018970654,0.0012972758,0.00046175506,0.004792667],"category_scores_gemma":[0.0044012386,0.00038026588,0.00059520814,0.0029696373,0.0004907177,0.0011430619,0.0014972149,0.00071730855,0.0039247004],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027260534,0.00011314171,0.34268948,0.00019106918,0.00016294052,0.00011965267,0.0006323177,0.0042462633,0.02190137,0.009260871,0.022510398,0.59789985],"study_design_scores_gemma":[0.00007388201,0.00014180901,0.77800304,0.00011164822,0.00015491762,0.0010347514,0.00051897805,0.077371754,0.016881527,0.013944774,0.111577,0.0001859006],"about_ca_topic_score_codex":0.007504243,"about_ca_topic_score_gemma":0.009767587,"teacher_disagreement_score":0.007504243,"about_ca_system_score_codex":0.0007090474,"about_ca_system_score_gemma":0.00071162864,"threshold_uncertainty_score":0.016033053},"labels":[],"label_agreement":null},{"id":"W2090289070","doi":"10.1088/0004-637x/728/2/113","title":"IMPROVED ANALYTICAL DESCRIPTION OF PARALLEL DIFFUSION WITH ADIABATIC FOCUSING","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Laser-Plasma Interactions and Diagnostics","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Adiabatic process; Diffusion; Isotropy; Pitch angle; Order (exchange); Scattering; Classical mechanics; Statistical physics; Computational physics; Mathematical analysis; Optics; Quantum mechanics","score_opus":0.019751508933640374,"score_gpt":0.22862739675361998,"score_spread":0.20887588781997962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090289070","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.042374194,0.0026588833,0.91410726,0.00046600102,0.00021936656,0.000099957084,0.00017420243,0.00033723647,0.039562814],"genre_scores_gemma":[0.7668538,0.005175944,0.17828369,0.0003750938,0.0003513667,0.0002860503,0.00021108508,0.00032014126,0.048142705],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997795,0.00003528658,0.000010222431,0.000032599666,0.00010431863,0.00003808217],"domain_scores_gemma":[0.9996611,0.000103520804,0.00004328373,0.000056940386,0.000110352245,0.000024795923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057980954,0.00088956795,0.00058458804,0.0008652667,0.0004520506,0.0006664234,0.0014055577,0.000755573,0.0038706777],"category_scores_gemma":[0.0016580913,0.00029712645,0.00061932165,0.0005626517,0.00071990606,0.0018229245,0.001054479,0.0010488504,0.00076046184],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036560374,0.000035875808,0.00032044933,0.00014940686,0.000021671201,0.00046290268,0.00015055195,0.16137113,0.022538366,0.7958729,0.0020171485,0.017022962],"study_design_scores_gemma":[0.00000808496,0.000016066002,0.00016514117,0.0000147574665,0.000011311998,0.00019423863,0.000014915527,0.922664,0.002148667,0.07081553,0.003923691,0.000023599667],"about_ca_topic_score_codex":0.0024662192,"about_ca_topic_score_gemma":0.0014219235,"teacher_disagreement_score":0.0038706777,"about_ca_system_score_codex":0.0012576986,"about_ca_system_score_gemma":0.0009054371,"threshold_uncertainty_score":0.012948692},"labels":[],"label_agreement":null},{"id":"W2090315770","doi":"10.1088/0004-637x/693/1/677","title":"EFFECTS OF UNIFORM AND DIFFERENTIAL ROTATION ON STELLAR PULSATIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Saint Mary's University","funders":"","keywords":"Differential rotation; Rotation (mathematics); Stellar rotation; Rotation period; Differential (mechanical device); Stellar pulsation; Internal rotation","score_opus":0.00579755558486201,"score_gpt":0.21454117180131993,"score_spread":0.20874361621645793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090315770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99767524,0.00020651912,0.00047054281,0.000043325766,0.000024330266,0.0000065723148,0.00018009687,0.00003179593,0.0013615771],"genre_scores_gemma":[0.9989832,0.00011388959,0.0001118745,0.000031722237,0.000023250841,0.0000042001675,0.00017005303,0.000029656372,0.0005322021],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99961203,0.00012017761,0.000034508645,0.000095667405,0.0000338877,0.00010373503],"domain_scores_gemma":[0.9920059,0.0058017625,0.0004641142,0.00046001014,0.0003435564,0.0009247096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071365386,0.0004194901,0.0006931198,0.00048918935,0.00047017116,0.0007555438,0.000348208,0.0003984631,0.008105843],"category_scores_gemma":[0.008685743,0.00024059217,0.0004383681,0.0004595599,0.00076422247,0.0005219469,0.00130155,0.00048208426,0.00045719216],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.117299765,0.0016300817,0.47337082,0.00073677255,0.0008127139,0.0014075876,0.0007610972,0.029390031,0.27056947,0.0034723508,0.0013843436,0.099165045],"study_design_scores_gemma":[0.00070693775,0.0042388565,0.9534692,0.000039066865,0.0004379504,0.0005647929,0.0004078512,0.009499874,0.028196014,0.0015451709,0.0008363461,0.000057972735],"about_ca_topic_score_codex":0.0011261082,"about_ca_topic_score_gemma":0.0009386708,"teacher_disagreement_score":0.008105843,"about_ca_system_score_codex":0.0003654813,"about_ca_system_score_gemma":0.00018070234,"threshold_uncertainty_score":0.027116776},"labels":[],"label_agreement":null},{"id":"W2090385535","doi":"10.1086/321538","title":"Cosmological Evolution of Supergiant Star‐forming Clouds","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Supergiant; Galaxy; Dark matter; Star formation; Astronomy; Star cluster; Cold dark matter; Molecular cloud; Galaxy cluster; Galaxy formation and evolution; Stars","score_opus":0.00977843920209232,"score_gpt":0.21620522734461692,"score_spread":0.2064267881425246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090385535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996842,0.00011903177,0.0015393936,0.00012400869,0.0000020084303,0.000004012092,0.000036943733,0.000027558,0.0013050617],"genre_scores_gemma":[0.9987142,0.00009185741,0.0008350909,0.000014004732,0.0000023773705,0.0000020807345,0.000046145964,0.000009084289,0.00028516885],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992573,0.000026510226,0.0000023451114,0.000015350799,0.000014453966,0.00001558163],"domain_scores_gemma":[0.99959403,0.000110229776,0.00012501943,0.000035942336,0.000032955908,0.00010179257],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033396576,0.00018384767,0.00016728244,0.00045998264,0.0007538034,0.00086055003,0.0005106491,0.00044626943,0.0011106424],"category_scores_gemma":[0.0020594313,0.00025808858,0.00030883084,0.00043859752,0.0005489622,0.00069576997,0.00051875226,0.0003888115,0.000094328316],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017380918,0.00009805462,0.46974814,0.00006672767,0.0001713428,0.0008533822,0.0024940828,0.33813575,0.018131835,0.15757833,0.0008637431,0.011684839],"study_design_scores_gemma":[0.00006783152,0.00009730512,0.34404364,0.000026830638,0.000103144375,0.0003549306,0.000745667,0.59950703,0.0028772478,0.047948338,0.004147811,0.00008028014],"about_ca_topic_score_codex":0.021989902,"about_ca_topic_score_gemma":0.020840602,"teacher_disagreement_score":0.021989902,"about_ca_system_score_codex":0.0016686004,"about_ca_system_score_gemma":0.00048816254,"threshold_uncertainty_score":0.04372382},"labels":[],"label_agreement":null},{"id":"W2090405334","doi":"10.1086/591792","title":"Reconstructing the Guitar: Blowing Bubbles with a Pulsar Bow Shock Backflow","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Bow shock (aerodynamics); Pulsar; Heliosphere; Backflow; Nebula; Kinetic energy; Astrophysics; Ram pressure; Interstellar medium; Bow wave; Shock (circulatory); Mechanics; Shock wave; Classical mechanics; Solar wind; Plasma; Geology","score_opus":0.015741995306638744,"score_gpt":0.2768604653169071,"score_spread":0.2611184700102684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090405334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96590126,0.00037810314,0.029833207,0.00040665703,0.00004604812,0.00004561371,0.0005480728,0.0012990135,0.0015420225],"genre_scores_gemma":[0.9870892,0.00008402936,0.012028027,0.00003722069,0.000024925786,0.0000075592825,0.000383557,0.000057629844,0.00028785836],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999361,0.000011919763,0.0000030715362,0.000015607431,0.000015283269,0.000018032651],"domain_scores_gemma":[0.9996803,0.0001358971,0.000045878725,0.00003041931,0.000034891982,0.00007259017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026671984,0.00043236188,0.0004228937,0.0008928916,0.00027525023,0.0006573009,0.00060853333,0.0010924845,0.0020167574],"category_scores_gemma":[0.0015107004,0.00041732873,0.00033161105,0.00040667507,0.00031952755,0.0004338074,0.00065980665,0.00050761795,0.00022042407],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026990096,0.00037497934,0.18218477,0.0004072119,0.00047996597,0.014700313,0.0016460272,0.55382305,0.16224314,0.012030903,0.006560376,0.06285028],"study_design_scores_gemma":[0.0001519509,0.00013164572,0.034039367,0.00002243333,0.0000464265,0.000517361,0.00017847473,0.955498,0.004798125,0.0033560568,0.0012259204,0.00003428941],"about_ca_topic_score_codex":0.0060711107,"about_ca_topic_score_gemma":0.0047636633,"teacher_disagreement_score":0.0060711107,"about_ca_system_score_codex":0.0003694135,"about_ca_system_score_gemma":0.0002741087,"threshold_uncertainty_score":0.01207155},"labels":[],"label_agreement":null},{"id":"W2090428815","doi":"10.1088/0004-637x/756/1/71","title":"CLUSTERING PROPERTIES OF B<i>z</i>K-SELECTED GALAXIES IN GOODS-N: ENVIRONMENTAL QUENCHING AND TRIGGERING OF STAR FORMATION AT<i>z</i>∼ 2","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"Centre National de la Recherche Scientifique; National Science Council; Science and Technology Facilities Council; National Science Foundation","keywords":"Astrophysics; Physics; Galaxy; Stellar mass; Star formation; Redshift; Correlation function (quantum field theory); Astronomy","score_opus":0.00846537908185534,"score_gpt":0.18483688640902418,"score_spread":0.17637150732716883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090428815","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995758,0.00001889047,0.000033834185,0.0000041970475,2.4545133e-7,0.0000016088367,0.00012620067,0.000004131194,0.00023508887],"genre_scores_gemma":[0.9993554,0.000010400548,0.0000386285,0.0000037379998,7.1616023e-7,0.0000017383462,0.00044970983,0.0000020504203,0.00013770178],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986863,0.0000118105045,0.00000820285,0.00004371035,0.000020773716,0.000046905545],"domain_scores_gemma":[0.9993718,0.00005664599,0.0002454758,0.000056031768,0.00008875085,0.0001813773],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001519536,0.00014723845,0.00024435183,0.0010526758,0.00025320007,0.00048327332,0.00026110167,0.00022098277,0.0009686065],"category_scores_gemma":[0.0005355625,0.00016725756,0.00017046416,0.000702648,0.00033575814,0.00017579888,0.0004430214,0.00016189153,0.00038967704],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012324029,0.000022412796,0.9907872,0.000006684978,0.000023237842,0.000034543347,0.0002262734,0.00022808702,0.007199998,0.00007509684,0.00008079838,0.0011923787],"study_design_scores_gemma":[8.984865e-7,0.0000061516985,0.9996853,4.791644e-7,0.0000023219156,0.000014164412,0.000043579144,0.00010748309,0.00010518658,0.0000066278335,0.000026764124,9.058997e-7],"about_ca_topic_score_codex":0.018651923,"about_ca_topic_score_gemma":0.028669747,"teacher_disagreement_score":0.018651923,"about_ca_system_score_codex":0.0004490759,"about_ca_system_score_gemma":0.00011335419,"threshold_uncertainty_score":0.037086725},"labels":[],"label_agreement":null},{"id":"W2090642949","doi":"10.1086/587514","title":"Mass Accretion Rates in Self-Regulated Disks of T Tauri Stars","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Saint Mary's University","funders":"","keywords":"T Tauri star; Physics; Astrophysics; Accretion (finance); Stars; Amplitude; Accretion disc; Molecular cloud; Astronomy","score_opus":0.010923635681502723,"score_gpt":0.23787606433726793,"score_spread":0.2269524286557652,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090642949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99911207,0.000048474038,0.0004480263,0.00002477342,0.000001657691,0.0000020833686,0.000025810301,0.000010509222,0.0003265696],"genre_scores_gemma":[0.99945897,0.00002892464,0.00029559995,0.000006348213,0.0000018915996,0.0000041549974,0.000044531178,0.000005921679,0.00015353612],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998876,0.00002345193,0.000009699391,0.000026817244,0.000018327073,0.00003415169],"domain_scores_gemma":[0.99872214,0.0005756013,0.00033039539,0.00010898203,0.00013278128,0.00013010792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000412953,0.00030632512,0.0002991223,0.00050192175,0.0004348881,0.0009084157,0.00080069795,0.000731715,0.0005258705],"category_scores_gemma":[0.004299349,0.00037914232,0.00057319744,0.00038592983,0.00072279887,0.0008308541,0.00053140987,0.00041531044,0.00014491516],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032343983,0.00013632287,0.24419211,0.000073460906,0.0001798059,0.00091721286,0.00043005345,0.7198114,0.021033842,0.007561683,0.0002400412,0.005100623],"study_design_scores_gemma":[0.00009428254,0.00012887805,0.04973579,0.000013001991,0.000045843364,0.00026244353,0.00014471781,0.9424966,0.0046637496,0.0020952446,0.00029015794,0.00002931939],"about_ca_topic_score_codex":0.008420069,"about_ca_topic_score_gemma":0.0041625584,"teacher_disagreement_score":0.008420069,"about_ca_system_score_codex":0.001257552,"about_ca_system_score_gemma":0.0004604746,"threshold_uncertainty_score":0.01674211},"labels":[],"label_agreement":null},{"id":"W2090676685","doi":"10.1088/0004-637x/754/1/33","title":"THE VERY HIGH ENERGY EMISSION FROM PULSARS: A CASE FOR INVERSE COMPTON SCATTERING","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Compton scattering; Cherenkov radiation; Gamma ray; Photon; Luminosity; Astrophysics; Particle acceleration; Fermi Gamma-ray Space Telescope; Scattering; Nuclear physics; Optics; Detector; Plasma; Galaxy","score_opus":0.0167503954646418,"score_gpt":0.30356534427924353,"score_spread":0.28681494881460173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090676685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83546114,0.010509088,0.06476243,0.0043896907,0.0003393967,0.000049415376,0.00008571514,0.00039660028,0.08400652],"genre_scores_gemma":[0.9937874,0.0007381225,0.0024710915,0.00019106871,0.00011162139,0.00001468132,0.000020850548,0.000019596695,0.0026455226],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998547,0.00002872581,0.000004644018,0.000044442637,0.000032885655,0.000034551707],"domain_scores_gemma":[0.9995809,0.00024136911,0.000056620785,0.000058418125,0.000028156473,0.00003462694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031119888,0.00039766982,0.0002659492,0.0003560786,0.00047133406,0.0013956232,0.00050362066,0.0011021285,0.0018345035],"category_scores_gemma":[0.0009247873,0.00022082248,0.00023515892,0.00030883172,0.0016552088,0.0009266938,0.00064564095,0.000722459,0.00033154248],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024309791,0.0001371961,0.040644612,0.00030962558,0.000057348865,0.005964562,0.00089267845,0.014465723,0.039157443,0.8607223,0.0036921676,0.0337132],"study_design_scores_gemma":[0.00007908255,0.00029028658,0.036236014,0.00019960973,0.000035554753,0.009432921,0.0007525158,0.11875937,0.008758602,0.8074584,0.017931936,0.00006561059],"about_ca_topic_score_codex":0.00033570538,"about_ca_topic_score_gemma":0.00021233696,"teacher_disagreement_score":0.0018345035,"about_ca_system_score_codex":0.00034876546,"about_ca_system_score_gemma":0.00011643804,"threshold_uncertainty_score":0.006137073},"labels":[],"label_agreement":null},{"id":"W2090905385","doi":"10.1086/430373","title":"Detailed Spectroscopic and Photometric Analysis of DQ White Dwarfs","year":2005,"lang":"fr","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; White dwarf; Astrophysics; Astronomy; Light curve; Photometry (optics); Stars","score_opus":0.009539363025455364,"score_gpt":0.23527048615496732,"score_spread":0.22573112312951196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090905385","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99157715,0.00027690982,0.0028551752,0.000020898191,0.000005230106,0.000011666634,0.003229251,0.00008418663,0.0019396691],"genre_scores_gemma":[0.99381304,0.000092984745,0.0013374406,0.00001452501,0.00000783623,0.000005375853,0.0040096613,0.000022495573,0.00069661456],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998043,0.00003206623,0.000013648581,0.000058965103,0.00006405957,0.000026932777],"domain_scores_gemma":[0.9993155,0.000090792106,0.00016319093,0.0001148554,0.0002101092,0.00010553444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004866516,0.00025912563,0.00022392797,0.0019910992,0.0004608112,0.00029420442,0.00014306548,0.00011193025,0.0008511405],"category_scores_gemma":[0.0006733387,0.00012221759,0.00019676077,0.0012257431,0.0001665589,0.00016965422,0.00030179947,0.00014080881,0.00042183077],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013033586,0.00003845768,0.9482997,0.00005332547,0.0000528075,0.00012867448,0.00026732066,0.0021886462,0.025390843,0.00058622734,0.0007583318,0.022105291],"study_design_scores_gemma":[0.000004571627,0.00003525903,0.9926473,0.0000028781628,0.000016367003,0.00015639975,0.000048005855,0.0014240108,0.002330493,0.00019162991,0.003138082,0.0000050023054],"about_ca_topic_score_codex":0.0073161605,"about_ca_topic_score_gemma":0.009415986,"teacher_disagreement_score":0.0073161605,"about_ca_system_score_codex":0.0003146497,"about_ca_system_score_gemma":0.00022624641,"threshold_uncertainty_score":0.014547169},"labels":[],"label_agreement":null},{"id":"W2090919784","doi":"10.1088/0004-637x/752/2/136","title":"COMET 22P/KOPFF: DUST ENVIRONMENT AND GRAIN EJECTION ANISOTROPY FROM VISIBLE AND INFRARED OBSERVATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency; Instituto de Astrofísica de Andalucía; Junta de Andalucía","keywords":"Comet; Cosmic dust; Infrared; Anisotropy; Outgassing; Interplanetary medium; Comet nucleus; Isotropy; Monte Carlo method","score_opus":0.015146070996951966,"score_gpt":0.20601505486730082,"score_spread":0.19086898387034884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090919784","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978405,0.0000844684,0.00065117574,0.0000252282,0.000002017235,0.0000054567195,0.0006532932,0.000073263225,0.0006645753],"genre_scores_gemma":[0.99813336,0.000041143634,0.0004997255,0.000007317943,0.000005004392,0.00000488599,0.0011892256,0.00001779082,0.00010165576],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999167,0.000007143133,0.000003153284,0.00002656883,0.000017219918,0.000029356921],"domain_scores_gemma":[0.99980074,0.000036680987,0.00007115278,0.000024519095,0.000028197283,0.000038666287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020092214,0.0003856345,0.00029457774,0.00054174924,0.0002680593,0.0005152792,0.00059231947,0.0003743805,0.00069857115],"category_scores_gemma":[0.0005436821,0.0002214128,0.00048096495,0.00043042473,0.00018122481,0.0003182719,0.00029620918,0.00018908139,0.0001762907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046321223,0.00011759091,0.75434244,0.00013378901,0.00032482448,0.001737577,0.00032381772,0.19006383,0.035642475,0.00086771004,0.001796641,0.014186078],"study_design_scores_gemma":[0.000028420853,0.000047740534,0.7905253,0.000010632095,0.000058210895,0.00029955216,0.00005056283,0.20422651,0.0037022384,0.00019539506,0.0008216743,0.000033718166],"about_ca_topic_score_codex":0.03365128,"about_ca_topic_score_gemma":0.03379694,"teacher_disagreement_score":0.03365128,"about_ca_system_score_codex":0.001340856,"about_ca_system_score_gemma":0.00026938308,"threshold_uncertainty_score":0.06691086},"labels":[],"label_agreement":null},{"id":"W2090941992","doi":"10.1088/0004-637x/697/1/293","title":"ANATOMY OF THE BAR INSTABILITY IN CUSPY DARK MATTER HALOS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Halo; Dark matter halo; Cuspy halo problem; Dark matter; Galactic halo; Instability","score_opus":0.005166899292015606,"score_gpt":0.2184247651784871,"score_spread":0.2132578658864715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090941992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9901329,0.00009578062,0.00515614,0.00012452586,0.000007231606,0.000014850637,0.0000724456,0.00006854179,0.004327565],"genre_scores_gemma":[0.99835396,0.000038468093,0.0010749847,0.000013717687,0.0000036084618,0.000008313344,0.000034251254,0.000018489682,0.00045421778],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999113,0.000030417577,0.0000037528202,0.000010848421,0.000017924238,0.000025788806],"domain_scores_gemma":[0.9996737,0.00007596055,0.000077453864,0.000034719742,0.000041552743,0.000096571195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025162424,0.00038218003,0.00031216073,0.0006316903,0.0005905561,0.00090628804,0.0006244099,0.00053016323,0.0015067375],"category_scores_gemma":[0.0010936023,0.00025752178,0.00061628193,0.00023013516,0.0007221929,0.00047263745,0.0010754111,0.00037667432,0.00016262116],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028324072,0.000092459544,0.042510774,0.000060176455,0.0000948734,0.0007623179,0.00046700792,0.9020068,0.018249782,0.03155453,0.0004743505,0.0034437503],"study_design_scores_gemma":[0.000052973923,0.00007878344,0.0073213275,0.000010237605,0.00001982869,0.00012113184,0.00011422949,0.9849924,0.0011554327,0.005685154,0.00042991436,0.0000185453],"about_ca_topic_score_codex":0.01107733,"about_ca_topic_score_gemma":0.005108766,"teacher_disagreement_score":0.01107733,"about_ca_system_score_codex":0.00092358404,"about_ca_system_score_gemma":0.00043466134,"threshold_uncertainty_score":0.022025764},"labels":[],"label_agreement":null},{"id":"W2090990268","doi":"10.1086/432710","title":"Equilibrium Disk‐Bulge‐Halo Models for the Milky Way and Andromeda Galaxies","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":253,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Queen's University","funders":"","keywords":"Physics; Andromeda; Bulge; Milky Way; Astrophysics; Andromeda Galaxy; Halo; Astronomy; Galaxy; Galactic halo","score_opus":0.011511161561806552,"score_gpt":0.2191198818673845,"score_spread":0.20760872030557792,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090990268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87970614,0.0012458466,0.099258505,0.00036057556,0.000043269418,0.00006559953,0.0009793583,0.00027863515,0.018061928],"genre_scores_gemma":[0.9830645,0.00042096555,0.010943383,0.000038027294,0.000020142706,0.00006615256,0.00030200568,0.000038859795,0.0051060054],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999032,0.00003443414,0.000006972527,0.00001775297,0.000018588493,0.00001913115],"domain_scores_gemma":[0.9998411,0.000043659034,0.00003950853,0.000020099795,0.000024397601,0.00003118353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019295707,0.00041886038,0.00044180217,0.00047251422,0.00046745638,0.0008089295,0.001607736,0.0006181172,0.0015588839],"category_scores_gemma":[0.00069966377,0.00039659577,0.00055280287,0.00025438063,0.0004117246,0.0008503246,0.0007771201,0.00040495256,0.00027566022],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009111219,0.00003906489,0.0067570857,0.000022875533,0.000055289747,0.00022219807,0.00023502839,0.89166844,0.0017078774,0.09417298,0.00059326726,0.004434836],"study_design_scores_gemma":[0.00007164365,0.00003207646,0.0025525424,0.000008753757,0.00002867929,0.00010974861,0.000062624305,0.96823835,0.0002681483,0.025076905,0.0035299049,0.000020551184],"about_ca_topic_score_codex":0.023776945,"about_ca_topic_score_gemma":0.019639583,"teacher_disagreement_score":0.023776945,"about_ca_system_score_codex":0.0011160541,"about_ca_system_score_gemma":0.0004483814,"threshold_uncertainty_score":0.047277093},"labels":[],"label_agreement":null},{"id":"W2090995106","doi":"10.1086/500726","title":"Nonlinear Hydromagnetic Wave Support of a Stratified Molecular Cloud. II. A Parameter Study","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Dimensionless quantity; Physics; Turbulence; Magnetohydrodynamics; Mechanics; Computational physics; Amplitude; Nonlinear system; Molecular cloud; Equation of state; Magnetic field; Statistical physics; Optics; Astrophysics; Thermodynamics","score_opus":0.009309328019043292,"score_gpt":0.2330362978091027,"score_spread":0.2237269697900594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2090995106","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974064,0.00005913501,0.00083442184,0.000059282047,0.00000492504,0.000011892705,0.000085222906,0.000015696423,0.0015230117],"genre_scores_gemma":[0.99953866,0.00003298562,0.00025472214,0.000010350867,0.000002310289,0.0000050276894,0.00003626512,0.0000048069714,0.00011498233],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999262,0.00001539256,0.000004155743,0.000008376989,0.00001427218,0.000031543506],"domain_scores_gemma":[0.9997141,0.00011717247,0.00006555921,0.000026726226,0.000031607753,0.000044925728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014376373,0.0003322842,0.00030108332,0.00036395437,0.00053275155,0.00080968643,0.0004824304,0.0005626013,0.0010062514],"category_scores_gemma":[0.0009325444,0.00015969982,0.00041097216,0.00022890618,0.00062330335,0.0004010348,0.0005249775,0.00041054885,0.000108656066],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034638212,0.00016147477,0.02896731,0.00008757891,0.00007061001,0.0008097906,0.00013978596,0.9215996,0.040346116,0.004932042,0.00022955559,0.0023097363],"study_design_scores_gemma":[0.0000396835,0.000087678876,0.00624561,0.000009047827,0.000016209173,0.000055725122,0.000064764514,0.98890764,0.0039302288,0.00047404855,0.00015880515,0.000010492601],"about_ca_topic_score_codex":0.010596468,"about_ca_topic_score_gemma":0.003989354,"teacher_disagreement_score":0.010596468,"about_ca_system_score_codex":0.00080425217,"about_ca_system_score_gemma":0.00042513476,"threshold_uncertainty_score":0.021069527},"labels":[],"label_agreement":null},{"id":"W2091049918","doi":"10.1088/0004-637x/788/1/78","title":"SPATIALLY RESOLVING THE VERY HIGH ENERGY EMISSION FROM MGRO J2019+37 WITH VERITAS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Vela; Supernova remnant; Spectral index; Point source; Astronomy; Observatory; Power law; Supernova; Astroparticle physics; Photon; Pulsar; Spectral line; Optics; Cosmic ray","score_opus":0.004282050432440117,"score_gpt":0.18015789628604031,"score_spread":0.1758758458536002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091049918","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9912368,0.0001713986,0.0006480973,0.00012917144,0.000013505993,0.000010184995,0.0009651038,0.00019560916,0.006630199],"genre_scores_gemma":[0.9921868,0.00014417792,0.0037699942,0.00009187715,0.000038076552,0.000008259091,0.0023261837,0.00006737445,0.001367309],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998379,0.0000052111245,0.0000052350233,0.00004077319,0.000050386738,0.000060423965],"domain_scores_gemma":[0.99976236,0.000018091298,0.000079104364,0.000046514677,0.000023010125,0.000070878465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014426137,0.00020688829,0.00022362436,0.0009136469,0.0003280828,0.0005830347,0.0004252483,0.00030277704,0.002818426],"category_scores_gemma":[0.00027800765,0.00024868562,0.00024670755,0.0005833699,0.00025195337,0.00027260336,0.0006394894,0.00027523213,0.0005793952],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069430156,0.00017069998,0.21422333,0.0001299939,0.00019349666,0.0042257938,0.0005354867,0.003537539,0.7278166,0.0014313896,0.0041587837,0.042882696],"study_design_scores_gemma":[0.000101601065,0.00019793438,0.9435357,0.000047316338,0.00012326555,0.0027198272,0.00037184174,0.008198252,0.03106015,0.0005561609,0.013051336,0.000036578927],"about_ca_topic_score_codex":0.009199116,"about_ca_topic_score_gemma":0.026468951,"teacher_disagreement_score":0.009199116,"about_ca_system_score_codex":0.0005384768,"about_ca_system_score_gemma":0.00033606176,"threshold_uncertainty_score":0.018291116},"labels":[],"label_agreement":null},{"id":"W2091050247","doi":"10.1088/0004-637x/756/2/170","title":"FORMING AN O STAR VIA DISK ACCRETION?","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Outflow; Physics; Astrophysics; Submillimeter Array; Protostar; Bipolar outflow; Accretion (finance); Velocity gradient; Rotation (mathematics); Perpendicular; Star formation; Emission spectrum; Astronomy; Spectral line; Geometry; Stars; Mechanics","score_opus":0.012970430761694096,"score_gpt":0.259028687518271,"score_spread":0.24605825675657692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091050247","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99298817,0.0007887539,0.0004095519,0.00012478398,0.000014564087,0.000014815477,0.000074920645,0.000013665666,0.005570806],"genre_scores_gemma":[0.9971636,0.0004499888,0.00045563304,0.00010202655,0.00002404796,0.0000057185516,0.00013534803,0.0000043978575,0.0016592279],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99988914,0.000015176091,0.0000055727373,0.000029030405,0.000017232227,0.000043738062],"domain_scores_gemma":[0.999843,0.000016849352,0.000057526526,0.000018148696,0.000011677474,0.000052682386],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019008135,0.00021359407,0.00030404056,0.00028864606,0.0008189813,0.0009483407,0.00030492796,0.0004469962,0.0019402575],"category_scores_gemma":[0.0005958598,0.00012718012,0.00016301176,0.00044407125,0.00039961384,0.0005095799,0.00072409253,0.00022617588,0.0010598904],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045613956,0.00031424608,0.9098995,0.000076981414,0.000048970454,0.006453285,0.0011995183,0.00049602025,0.011097737,0.0028315613,0.0013354962,0.06579056],"study_design_scores_gemma":[0.00008219306,0.0011499501,0.9271786,0.000054649143,0.000082235165,0.016409628,0.0034466456,0.006093966,0.0034425654,0.005517239,0.036513418,0.000028846616],"about_ca_topic_score_codex":0.002271453,"about_ca_topic_score_gemma":0.0026185764,"teacher_disagreement_score":0.002271453,"about_ca_system_score_codex":0.0002994347,"about_ca_system_score_gemma":0.0001704349,"threshold_uncertainty_score":0.006490767},"labels":[],"label_agreement":null},{"id":"W2091071161","doi":"10.1086/507175","title":"Diffuse, Nonthermal X‐Ray Emission from the Galactic Star Cluster Westerlund 1","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Supernova; Luminosity; Stars; Flux (metallurgy); Electron; Cluster (spacecraft); Emission spectrum; Galaxy; Astronomy; Spectral line; Nuclear physics","score_opus":0.00913513466170831,"score_gpt":0.2155558296392227,"score_spread":0.2064206949775144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091071161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976792,0.0003987547,0.00020461263,0.000012753397,0.0000066168736,0.000005619616,0.00026396927,0.00003714016,0.0013912579],"genre_scores_gemma":[0.9957955,0.00054970075,0.0011938238,0.000020716572,0.000017981953,0.000007901484,0.001249053,0.000021001952,0.0011443971],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999025,0.000002881552,0.0000034975017,0.000034857225,0.000026198488,0.000030051471],"domain_scores_gemma":[0.9998271,0.000011058586,0.0000557769,0.000019382898,0.000022910777,0.00006381627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000094427756,0.0003270164,0.00029977376,0.0010864555,0.00047356487,0.00070540456,0.00038173687,0.0001749509,0.0009600322],"category_scores_gemma":[0.0001853291,0.00020443788,0.00014119348,0.0007467627,0.00021372222,0.00025676985,0.0006408707,0.00018634886,0.00033927656],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014304601,0.0002153633,0.5888914,0.0005140618,0.00019909343,0.003029672,0.0017822068,0.0019343006,0.35156244,0.0018353726,0.0034233532,0.04518225],"study_design_scores_gemma":[0.000021561804,0.00012373776,0.9809368,0.000022766288,0.00003873437,0.0011107166,0.00018879831,0.0009966055,0.009638443,0.00013054622,0.006769328,0.000021890619],"about_ca_topic_score_codex":0.009989949,"about_ca_topic_score_gemma":0.023760222,"teacher_disagreement_score":0.009989949,"about_ca_system_score_codex":0.0005723772,"about_ca_system_score_gemma":0.0002309511,"threshold_uncertainty_score":0.019863605},"labels":[],"label_agreement":null},{"id":"W2091088212","doi":"10.1088/0004-637x/793/2/88","title":"A BROADBAND X-RAY STUDY OF THE GEMINGA PULSAR WITH<i>NuSTAR</i>AND<i>XMM-NEWTON</i>","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Fonds Québécois de la Recherche sur la Nature et les Technologies; National Aeronautics and Space Administration; California Institute of Technology; Canada Research Chairs; Canadian Institute for Advanced Research","keywords":"Flattening; Pulsar; Black-body radiation; Spectral line; Broadband; Spectral index; Component (thermodynamics); Spectral analysis; Spectral shape analysis","score_opus":0.007378188287391859,"score_gpt":0.2069558570900966,"score_spread":0.19957766880270472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091088212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99764913,0.000278012,0.00081608846,0.000022527382,0.0000050096737,0.000007241322,0.000096489755,0.000033869732,0.0010916899],"genre_scores_gemma":[0.99674016,0.00016298504,0.0023202754,0.000058403737,0.000018818297,0.000006393835,0.0003830784,0.0000149031885,0.0002950068],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99988925,0.000011367323,0.0000071657123,0.000046374273,0.000022724098,0.000023072906],"domain_scores_gemma":[0.99948585,0.000085032916,0.00020823423,0.00006298316,0.00006433157,0.00009353656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032464036,0.0003949736,0.0002616175,0.00078299653,0.00055305375,0.0003945209,0.00032374405,0.00050288625,0.0005347357],"category_scores_gemma":[0.00047125615,0.00032117037,0.00031651236,0.0005462538,0.00026991373,0.00052944466,0.00046538454,0.00040388657,0.00030145384],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034275453,0.0002248196,0.35030967,0.00012673961,0.0001588589,0.0010105345,0.00045282816,0.0006259684,0.63007504,0.0004143313,0.00020935925,0.01604907],"study_design_scores_gemma":[0.000010015488,0.00058639084,0.97684675,0.000018458937,0.000066799636,0.0022231315,0.00014935528,0.0013861357,0.01645271,0.00020537117,0.002041109,0.000013775238],"about_ca_topic_score_codex":0.0005015836,"about_ca_topic_score_gemma":0.001047688,"teacher_disagreement_score":0.00078299653,"about_ca_system_score_codex":0.00017964748,"about_ca_system_score_gemma":0.00008296958,"threshold_uncertainty_score":0.0017889142},"labels":[],"label_agreement":null},{"id":"W2091102788","doi":"10.1088/0004-637x/693/1/l6","title":"THE PHYSICS OF CRYSTALLIZATION FROM GLOBULAR CLUSTER WHITE DWARF STARS IN NGC 6397","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Fonds Québécois de la Recherche sur la Nature et les Technologies; National Science Foundation","keywords":"Globular cluster; Physics; Astrophysics; Stars; White dwarf; Astronomy; Photometry (optics); Proper motion; Hubble space telescope; Crystallization; Blue straggler","score_opus":0.008184902464740918,"score_gpt":0.2173750331702576,"score_spread":0.2091901307055167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091102788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987696,0.00006474816,0.0003360532,0.000021969574,5.6195086e-7,0.000001293733,0.00005141788,0.000016666329,0.0007377549],"genre_scores_gemma":[0.99954116,0.000049066268,0.00019425231,0.0000051787665,0.0000018852445,0.0000013111968,0.000103472965,0.000007869349,0.00009581401],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999608,0.0000028716681,0.0000020238497,0.000007997804,0.000013342232,0.000012947802],"domain_scores_gemma":[0.9997807,0.000072463,0.000066479355,0.00002246448,0.000019975862,0.000037817797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001496448,0.00014122875,0.00030083483,0.00068978115,0.0006174007,0.00065076904,0.00022978018,0.0001867496,0.0004726843],"category_scores_gemma":[0.0005469311,0.00013281732,0.00023406572,0.00074608694,0.00073952967,0.0003964113,0.0006840429,0.00030825665,0.00008697209],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004911207,0.000075910306,0.60372835,0.00014078945,0.00011236708,0.0039444524,0.0039693047,0.058256876,0.2625701,0.04546652,0.0009932778,0.02025094],"study_design_scores_gemma":[0.00007019703,0.00009341185,0.84401697,0.0000332181,0.00006192768,0.0008170687,0.0007771685,0.083918676,0.026947532,0.04118224,0.0020327105,0.000048913487],"about_ca_topic_score_codex":0.007962914,"about_ca_topic_score_gemma":0.0074435696,"teacher_disagreement_score":0.007962914,"about_ca_system_score_codex":0.0010332351,"about_ca_system_score_gemma":0.00027550806,"threshold_uncertainty_score":0.01583314},"labels":[],"label_agreement":null},{"id":"W2091163781","doi":"10.1088/0004-637x/778/1/2","title":"VALIDATION OF THE EQUILIBRIUM MODEL FOR GALAXY EVOLUTION TO<i>z</i>∼ 3 THROUGH MOLECULAR GAS AND DUST OBSERVATIONS OF LENSED STAR-FORMING GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":272,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Galaxy; Luminous infrared galaxy; Star formation; Redshift; Astronomy; Plateau de Bure Interferometer; Galaxy formation and evolution; Peculiar galaxy; Lenticular galaxy","score_opus":0.01863134413967034,"score_gpt":0.22411070092440946,"score_spread":0.2054793567847391,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091163781","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95206547,0.00028915686,0.041529097,0.00019266264,0.000013857455,0.00006952,0.0009575323,0.0002420925,0.0046406374],"genre_scores_gemma":[0.9948837,0.00007701799,0.0038908736,0.000057045712,0.000008680503,0.00003701695,0.00056902133,0.000057883073,0.00041859705],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995572,0.00009735441,0.000018525068,0.00017488266,0.000064205,0.000087802444],"domain_scores_gemma":[0.9977749,0.0008458847,0.00032262143,0.00028115747,0.0004710725,0.0003044723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016919747,0.00051778916,0.0004761297,0.0008272779,0.0005683773,0.0011568707,0.0017605309,0.00060008094,0.0023148442],"category_scores_gemma":[0.0049859965,0.00028951425,0.00073961343,0.0003663703,0.00068549626,0.0013303687,0.0008567178,0.00049974886,0.00078553637],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006909717,0.0001709387,0.8106664,0.00011702285,0.00030643804,0.00022262696,0.00056058797,0.109424576,0.023297317,0.03179123,0.0008205034,0.021931404],"study_design_scores_gemma":[0.000121962956,0.00026130961,0.3709751,0.000031925752,0.00008646118,0.00021046035,0.00035900262,0.58798295,0.0075760237,0.029437438,0.0028837593,0.00007360117],"about_ca_topic_score_codex":0.03776343,"about_ca_topic_score_gemma":0.01574741,"teacher_disagreement_score":0.03776343,"about_ca_system_score_codex":0.0019129069,"about_ca_system_score_gemma":0.0011598582,"threshold_uncertainty_score":0.07508719},"labels":[],"label_agreement":null},{"id":"W2091234497","doi":"10.1086/521094","title":"Stellar Kinematics in the Complicated Inner Spheroid of M31: Discovery of Substructure along the Southeastern Minor Axis and Its Relationship to the Giant Southern Stream","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Red-giant branch; Astrophysics; Stellar kinematics; Astronomy; Radial velocity; Galaxy; Milky Way; Local Group; Stars; Population; Andromeda Galaxy; Velocity dispersion; Giant star; Satellite galaxy; Stellar population; Metallicity; Red giant; Star formation","score_opus":0.012026846838910914,"score_gpt":0.22068371261606196,"score_spread":0.20865686577715103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091234497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937016,0.00008331118,0.0002155765,0.000007084759,4.430788e-7,0.0000015557349,0.000025371739,0.0000063510943,0.00029025265],"genre_scores_gemma":[0.9993818,0.000053198222,0.0003632732,0.000004783765,0.00000276759,0.0000012422058,0.000081426624,0.0000018316867,0.000109728775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995005,0.0000063928683,0.0000033203328,0.000019206343,0.000010903586,0.000010191602],"domain_scores_gemma":[0.9996784,0.000042490734,0.00015325614,0.000042335658,0.000026338024,0.000057197005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012848819,0.00018263163,0.00014685917,0.00058695866,0.00029157932,0.00033104498,0.00017797612,0.00021047969,0.0006995801],"category_scores_gemma":[0.00033620518,0.00009099171,0.00012821525,0.0004512276,0.00026966215,0.00019362905,0.000406983,0.00012892904,0.00038980073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000110778965,0.000017007858,0.9241809,0.000016888673,0.000016707283,0.0005310961,0.00032934174,0.00032990365,0.063187666,0.00019932589,0.000063036154,0.011017368],"study_design_scores_gemma":[0.0000029205237,0.000074002084,0.99528116,0.0000029334872,0.000009926642,0.0013058227,0.00008103748,0.00053893897,0.0021623878,0.00011141156,0.0004254704,0.0000038951293],"about_ca_topic_score_codex":0.0015523871,"about_ca_topic_score_gemma":0.0023567853,"teacher_disagreement_score":0.0015523871,"about_ca_system_score_codex":0.00015075071,"about_ca_system_score_gemma":0.00011217985,"threshold_uncertainty_score":0.0030867457},"labels":[],"label_agreement":null},{"id":"W2091286088","doi":"10.1086/377479","title":"Intrinsic, Observed, and Retrieved Properties of Interstellar Turbulence","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Turbulence; Astrophysics; Scaling; Interstellar medium; Molecular cloud; Magnetohydrodynamics; Line (geometry); Principal component analysis; Shock (circulatory); Centroid; Computational physics; Statistical physics; Galaxy; Plasma; Stars; Mechanics; Statistics; Geometry","score_opus":0.023369954105562175,"score_gpt":0.21084820965380316,"score_spread":0.187478255548241,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091286088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7055765,0.0047072168,0.0084882965,0.017270014,0.02129683,0.00092278875,0.026236314,0.0029526397,0.21254943],"genre_scores_gemma":[0.79343814,0.0017532349,0.0027897912,0.0007024267,0.0063842605,0.0001693173,0.01357762,0.0007932447,0.180392],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9982406,0.00015654358,0.0001642637,0.00025131684,0.0010468899,0.00014052831],"domain_scores_gemma":[0.96105623,0.0039572474,0.0016845228,0.002329876,0.028931238,0.0020409268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016602388,0.00027750712,0.00074990117,0.0016987077,0.0011679182,0.0015809776,0.000796788,0.0011593015,0.0661969],"category_scores_gemma":[0.023806265,0.00020435758,0.00032903723,0.000919325,0.00045160693,0.0013028986,0.00079553586,0.00044449474,0.0222482],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018343066,0.00030986944,0.14923552,0.0028291468,0.00021109507,0.0032691273,0.0009966221,0.0010533477,0.047212493,0.0027486407,0.40448517,0.38581467],"study_design_scores_gemma":[0.0003359707,0.00059264875,0.51836514,0.0004016961,0.00036637808,0.0039554345,0.0018978934,0.0103097,0.052324276,0.0031190852,0.4080847,0.0002470591],"about_ca_topic_score_codex":0.0009234704,"about_ca_topic_score_gemma":0.0021925713,"teacher_disagreement_score":0.0661969,"about_ca_system_score_codex":0.00048137663,"about_ca_system_score_gemma":0.0009884749,"threshold_uncertainty_score":0.22145069},"labels":[],"label_agreement":null},{"id":"W2091304485","doi":"10.1088/0004-637x/785/1/11","title":"PROPERTIES OF M31. IV. CANDIDATE LUMINOUS BLUE VARIABLES FROM PANDROMEDA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Queen's University Belfast; National Aeronautics and Space Administration; California Institute of Technology; Queen's University; Johns Hopkins University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; Galaxy; Stars; Sky; Andromeda Galaxy; Spiral galaxy; Astronomy; Andromeda; Milky Way","score_opus":0.00985791537601129,"score_gpt":0.19331503723931354,"score_spread":0.18345712186330224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091304485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99845743,0.00013825556,0.00013941502,0.000017503035,0.000001963389,0.0000074669924,0.00042002558,0.000010829797,0.0008072066],"genre_scores_gemma":[0.99686384,0.00006569265,0.00037973648,0.00001011412,0.0000065084373,0.000008533048,0.0023232445,0.0000072895004,0.00033500264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998223,0.000017847015,0.00001568418,0.00006104509,0.000040794916,0.000042334403],"domain_scores_gemma":[0.9994863,0.00005123717,0.00021707569,0.00006058849,0.00006804213,0.00011664823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025667658,0.00027498035,0.00024268686,0.0021885305,0.000628188,0.00054572197,0.000270636,0.0001799029,0.0014083118],"category_scores_gemma":[0.0005683226,0.000102208,0.00021578105,0.0015424349,0.00017257122,0.00035038582,0.0006657407,0.00017003916,0.0005254118],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008765152,0.000034614433,0.9823137,0.000017794024,0.000019510677,0.0002169574,0.00017328987,0.00014194097,0.007425127,0.000110944435,0.00026840428,0.009190143],"study_design_scores_gemma":[0.0000024746485,0.000030487723,0.99813384,0.0000026561438,0.000005240305,0.00026879128,0.000083632935,0.00024191801,0.0004884001,0.00003122894,0.0007087936,0.0000025790994],"about_ca_topic_score_codex":0.0043480946,"about_ca_topic_score_gemma":0.007981192,"teacher_disagreement_score":0.0043480946,"about_ca_system_score_codex":0.0002160423,"about_ca_system_score_gemma":0.00012325429,"threshold_uncertainty_score":0.008645594},"labels":[],"label_agreement":null},{"id":"W2091331320","doi":"10.1086/337985","title":"The Star Formation History of the Large Magellanic Cloud","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Large Magellanic Cloud; Star formation; Stellar evolution; Luminosity; Stars; Hertzsprung–Russell diagram; Stellar density; Bar (unit); Star count","score_opus":0.012046852460929435,"score_gpt":0.20206161961095953,"score_spread":0.1900147671500301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091331320","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936528,0.00019279936,0.00086299377,0.00004220028,0.0000035693538,0.00001289445,0.0030752714,0.00004426712,0.002113183],"genre_scores_gemma":[0.9968304,0.000060538354,0.00075365626,0.000008000606,0.0000057425736,0.000003451535,0.0019750476,0.000005327835,0.00035780208],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992156,0.000011217063,0.0000033296715,0.00002815694,0.0000164916,0.000019305913],"domain_scores_gemma":[0.99951136,0.00009858901,0.00013703415,0.000059938848,0.00006416313,0.00012889321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026550228,0.00017302763,0.00012211042,0.001033371,0.0004200053,0.00033936728,0.0002469756,0.00012968028,0.001655758],"category_scores_gemma":[0.00073042396,0.000090371,0.00013647939,0.0010843369,0.00013847295,0.00037584934,0.00028014873,0.00019009967,0.0002620771],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012572794,0.00006435968,0.93366015,0.00005721698,0.00006826283,0.00032439025,0.0005653717,0.004696533,0.023403388,0.0010443754,0.000997507,0.034992673],"study_design_scores_gemma":[0.000004163093,0.000016999235,0.9938113,0.0000042277934,0.00000935348,0.00008262754,0.000030078645,0.0022226765,0.0013494907,0.00014893184,0.0023141832,0.000005942923],"about_ca_topic_score_codex":0.053563017,"about_ca_topic_score_gemma":0.073937416,"teacher_disagreement_score":0.053563017,"about_ca_system_score_codex":0.0008896429,"about_ca_system_score_gemma":0.0004234835,"threshold_uncertainty_score":0.10650253},"labels":[],"label_agreement":null},{"id":"W2091355548","doi":"10.1086/386299","title":"A Strong, Broad Absorption Feature in the X‐Ray Spectrum of the Nearby Neutron Star RX J1605.3+3249","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Neutron star; Physics; Astrophysics; Black-body radiation; Absorption (acoustics); Spectral line; Neutron; Atomic physics; Astronomy; Nuclear physics; Radiation; Optics","score_opus":0.009551069582361026,"score_gpt":0.22436710550579425,"score_spread":0.21481603592343324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091355548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99802125,0.00012181405,0.00019352697,0.000021840828,0.000004433566,0.0000022933139,0.0000656652,0.000018954008,0.0015501734],"genre_scores_gemma":[0.99895287,0.00006596014,0.0003224053,0.000024870118,0.000007744403,0.0000024227404,0.0001466595,0.0000050929116,0.00047189006],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996626,0.0000028096192,0.0000025058837,0.000011304477,0.0000092421205,0.0000078027415],"domain_scores_gemma":[0.9999187,0.0000077941595,0.000035985224,0.000006741785,0.0000071283393,0.000023640907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006704242,0.00017412394,0.0002174594,0.00035920425,0.00030463564,0.00024676448,0.00017334486,0.0002802882,0.001251272],"category_scores_gemma":[0.00012414069,0.000089803514,0.00014312538,0.00025510465,0.00020539353,0.00015306156,0.00029712162,0.00018941429,0.00026723937],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045967638,0.00014552522,0.1845508,0.0001810046,0.000104435036,0.0021368447,0.00043698327,0.0012129897,0.79096645,0.0014265751,0.0008253234,0.017553419],"study_design_scores_gemma":[0.00003091418,0.00022273732,0.97392535,0.000023487897,0.000039963175,0.0023130502,0.00013735254,0.0016087347,0.018960653,0.00040677763,0.0023204116,0.000010568123],"about_ca_topic_score_codex":0.00046326194,"about_ca_topic_score_gemma":0.0008133364,"teacher_disagreement_score":0.001251272,"about_ca_system_score_codex":0.00009222445,"about_ca_system_score_gemma":0.000049937524,"threshold_uncertainty_score":0.0041859746},"labels":[],"label_agreement":null},{"id":"W2091391324","doi":"10.1086/444358","title":"Whims of an Accreting Young Brown Dwarf: Exploring the Emission-Line Variability of 2MASSW J1207334-393254","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Brown dwarf; Accretion (finance); T Tauri star; Spectral line; Emission spectrum; Astronomy; Stars; Redshift; Line (geometry); Galaxy","score_opus":0.024236432923778053,"score_gpt":0.2620540050660084,"score_spread":0.23781757214223034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091391324","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99858344,0.00012541571,0.00021361433,0.000027255574,0.0000055758837,0.000003099016,0.00066272373,0.000035929115,0.0003429116],"genre_scores_gemma":[0.99436617,0.00008581638,0.0010026032,0.00004722641,0.000025753683,0.000009427158,0.0040443,0.000039435407,0.0003792627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998505,0.00001258768,0.0000072497464,0.0000559457,0.00003844201,0.000035116864],"domain_scores_gemma":[0.9996092,0.000038477177,0.00010894939,0.000041401458,0.00007738625,0.00012470174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037435978,0.0002282985,0.0003690175,0.0011128538,0.00047571573,0.0005756683,0.0002941593,0.00030146906,0.00042814456],"category_scores_gemma":[0.00045749705,0.00015278305,0.00028467696,0.00077024073,0.00023433234,0.00031814087,0.0005590852,0.00022867668,0.00031570136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025210605,0.0001138189,0.90365326,0.000073898205,0.00014820213,0.0008147916,0.0011532031,0.00062603084,0.07367504,0.00014335422,0.002128106,0.017218173],"study_design_scores_gemma":[0.0000047632743,0.000041354357,0.9958663,0.000007467842,0.000022476683,0.00024202351,0.00030208024,0.00074436486,0.00091622653,0.00005771744,0.0017876808,0.00000754002],"about_ca_topic_score_codex":0.008934614,"about_ca_topic_score_gemma":0.027999505,"teacher_disagreement_score":0.008934614,"about_ca_system_score_codex":0.00027949057,"about_ca_system_score_gemma":0.00021294867,"threshold_uncertainty_score":0.017765224},"labels":[],"label_agreement":null},{"id":"W2091485165","doi":"10.1086/320980","title":"The White Dwarf Distance to the Globular Cluster 47 Tucanae and Its Age","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Globular cluster; Physics; Astrophysics; White dwarf; Parallax; Sequence (biology); Cluster (spacecraft); Distance modulus; Astronomy; Stars; Chemistry","score_opus":0.008779969980539544,"score_gpt":0.2211553343763952,"score_spread":0.21237536439585566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091485165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9875573,0.0032976859,0.0016716202,0.00011835584,0.000033102435,0.0000056838385,0.00061179296,0.00007500632,0.00662956],"genre_scores_gemma":[0.995858,0.0005895895,0.0016689881,0.000018587594,0.00003796139,0.0000045504007,0.0006447932,0.000019399413,0.0011580816],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998499,0.0000067232922,0.0000039831984,0.00005704779,0.00004916139,0.000033305238],"domain_scores_gemma":[0.99940145,0.00007246508,0.0001856945,0.00004516553,0.00020016247,0.0000949729],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023098523,0.0002422333,0.0002519255,0.0019524123,0.00080223684,0.0007658336,0.0005921459,0.00045471863,0.0010140099],"category_scores_gemma":[0.0011954097,0.000112506044,0.0001249946,0.0011661024,0.00049341115,0.0005959947,0.00062876515,0.0003845477,0.0002933787],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016295972,0.000025269452,0.90664613,0.00007531671,0.00010079259,0.00028867472,0.0006961155,0.004079339,0.01634829,0.0028716135,0.0019415288,0.06676397],"study_design_scores_gemma":[0.0000052377377,0.000024796962,0.9799733,0.00001796535,0.00004142299,0.00036016264,0.00015313482,0.0041097244,0.0039534713,0.00073369755,0.010601848,0.000025274585],"about_ca_topic_score_codex":0.08820546,"about_ca_topic_score_gemma":0.13068151,"teacher_disagreement_score":0.08820546,"about_ca_system_score_codex":0.0018370706,"about_ca_system_score_gemma":0.00066376216,"threshold_uncertainty_score":0.1753841},"labels":[],"label_agreement":null},{"id":"W2091487047","doi":"10.1086/432875","title":"Dust Extinction in Compact Planetary Nebulae","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Extinction (optical mineralogy); Planetary nebula; Cosmic dust; Ionization; Shell (structure); Line (geometry); Orientation (vector space)","score_opus":0.012177067080021534,"score_gpt":0.22597289571080592,"score_spread":0.2137958286307844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091487047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99855536,0.00021924125,0.00061660697,0.000008794045,9.0075673e-7,0.0000018828949,0.00002020617,0.000011412392,0.0005654945],"genre_scores_gemma":[0.99968374,0.000065961154,0.00015062543,0.0000035326889,0.0000014315093,7.754864e-7,0.000032857246,0.0000030134383,0.000058006746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998988,0.000016557127,0.0000056868626,0.00003311598,0.000035091776,0.000010787355],"domain_scores_gemma":[0.9995454,0.00015039777,0.00015352377,0.00005767076,0.00004636244,0.000046635425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002550952,0.00014279276,0.00016262983,0.00038175273,0.00018562675,0.00044040827,0.0002126419,0.00014490604,0.00041296912],"category_scores_gemma":[0.0016843653,0.00014490038,0.0001300224,0.0002398684,0.00040643086,0.0002799039,0.0004347772,0.0001405112,0.00007749035],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041196207,0.0000966204,0.7610769,0.000113831884,0.00014270109,0.0008342854,0.00053444796,0.03094003,0.16154253,0.0018116232,0.00036869402,0.042126324],"study_design_scores_gemma":[0.00002036725,0.000115717594,0.9677536,0.00001326598,0.00003272917,0.0009659025,0.00014091328,0.018364785,0.010516727,0.0014985501,0.00057012297,0.000007379547],"about_ca_topic_score_codex":0.0019538065,"about_ca_topic_score_gemma":0.0014310654,"teacher_disagreement_score":0.0019538065,"about_ca_system_score_codex":0.0003263611,"about_ca_system_score_gemma":0.00006240994,"threshold_uncertainty_score":0.0038847923},"labels":[],"label_agreement":null},{"id":"W2091516034","doi":"10.1086/317333","title":"Space Telescope Imaging Spectrograph Echelle Observations of NGC 4151: Variable Ionization of the Intrinsic UV Absorbers","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Space Telescope Imaging Spectrograph; Physics; Astrophysics; Spectrograph; Galaxy; Ionization; Emission spectrum; Absorption spectroscopy; Spectral line; Astronomy; Absorption (acoustics); Hubble space telescope; Optics; Ion","score_opus":0.0061940409301125985,"score_gpt":0.19191870499512353,"score_spread":0.18572466406501092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091516034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99524504,0.00008700778,0.00017619153,0.00006270577,0.000007960793,0.000009062675,0.0019448159,0.00009001695,0.0023772025],"genre_scores_gemma":[0.99292797,0.00010299678,0.0008042765,0.000046168338,0.000024312678,0.000008511135,0.0050001214,0.000018896506,0.0010667519],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998425,0.00001157852,0.000008050213,0.00004824733,0.000044572145,0.000044888675],"domain_scores_gemma":[0.9995098,0.000029182635,0.00016868986,0.00007309863,0.000048242775,0.0001708824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021244267,0.00030895308,0.00020681274,0.001490852,0.0007231685,0.00052334776,0.00033655053,0.00034714947,0.0017314975],"category_scores_gemma":[0.00038204034,0.00020172338,0.00020762597,0.0010519194,0.00019944063,0.00036583163,0.00056976726,0.00037887442,0.00046945957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046018622,0.00044218844,0.9088409,0.00009260044,0.00018948155,0.0014775806,0.0014368983,0.0025423921,0.052441694,0.00079919654,0.008000676,0.023276098],"study_design_scores_gemma":[0.000014435283,0.000046515703,0.9955135,0.000005447297,0.000018983186,0.00025998746,0.000080450234,0.0008738109,0.0013231267,0.000058738195,0.0017973185,0.000007641747],"about_ca_topic_score_codex":0.012538525,"about_ca_topic_score_gemma":0.03222695,"teacher_disagreement_score":0.012538525,"about_ca_system_score_codex":0.0004941372,"about_ca_system_score_gemma":0.00017292735,"threshold_uncertainty_score":0.024931073},"labels":[],"label_agreement":null},{"id":"W2091540744","doi":"10.1086/422905","title":"Mass‐Radius Constraints from a Pulse Shape Model for Hercules X‐1","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Neutron star; RADIUS; Emissivity; Pulse (music); Accretion (finance); Geometry; Astrophysics; Computational physics; Optics","score_opus":0.023311679318060087,"score_gpt":0.24448657698142623,"score_spread":0.22117489766336615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091540744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90030384,0.00036803025,0.071982026,0.00042064878,0.000042842817,0.0000554825,0.0005323918,0.00049724535,0.025797503],"genre_scores_gemma":[0.9921171,0.000111094334,0.003750042,0.00005632323,0.000029352044,0.000040835075,0.00027827738,0.0001083593,0.0035087296],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999112,0.000015000445,0.0000040258883,0.000020720245,0.00002557094,0.000023393624],"domain_scores_gemma":[0.99973816,0.00008146996,0.00006384706,0.00003801764,0.000044607128,0.000033842363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029317796,0.00051974977,0.0005013069,0.00034285712,0.0005055286,0.00090630277,0.0009437482,0.0007079489,0.0019860598],"category_scores_gemma":[0.0011985982,0.0003644884,0.00038531443,0.00033675836,0.00036711904,0.00046956295,0.00064745225,0.00043385313,0.000621996],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035154275,0.00005908362,0.021060728,0.0000645358,0.000046682286,0.0011529182,0.00033515744,0.87054455,0.020105623,0.06934568,0.002666063,0.014267487],"study_design_scores_gemma":[0.000055420347,0.000043487813,0.007192416,0.000007612768,0.000016115047,0.000271423,0.000037580907,0.98046196,0.0014636338,0.0092103975,0.0012201736,0.000019837375],"about_ca_topic_score_codex":0.007940575,"about_ca_topic_score_gemma":0.003252799,"teacher_disagreement_score":0.007940575,"about_ca_system_score_codex":0.0010371805,"about_ca_system_score_gemma":0.0004859056,"threshold_uncertainty_score":0.015788674},"labels":[],"label_agreement":null},{"id":"W2091663007","doi":"10.1088/0004-637x/774/2/128","title":"AN IMPRINT OF MOLECULAR CLOUD MAGNETIZATION IN THE MORPHOLOGY OF THE DUST POLARIZED EMISSION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":253,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Magnetization; Morphology (biology); Molecular cloud; Cosmic dust; Cloud computing; Polarization (electrochemistry)","score_opus":0.005627826197936817,"score_gpt":0.22674904630461334,"score_spread":0.22112122010667654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091663007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99422556,0.00021909043,0.0011730953,0.00017406982,0.000019370531,0.000003172359,0.000111233334,0.00006053722,0.004013953],"genre_scores_gemma":[0.9994622,0.00005480513,0.00010225987,0.000013980846,0.000016879245,8.553189e-7,0.000028958406,0.000016595985,0.0003035071],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996233,0.0000045018105,9.661078e-7,0.000011860125,0.000006720471,0.000013645896],"domain_scores_gemma":[0.99962413,0.00016127397,0.00006472894,0.00003217826,0.000046391433,0.00007128208],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011948106,0.00011306197,0.0001793001,0.00036941015,0.0002572597,0.00069758523,0.00019050048,0.0002940306,0.003435398],"category_scores_gemma":[0.00095371803,0.0001809613,0.00012904969,0.00023044365,0.0004161361,0.00047323704,0.000328651,0.00040013628,0.000353018],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010534464,0.000120982084,0.12390311,0.00008481418,0.000059138623,0.0008459087,0.00040194055,0.0029033944,0.8381889,0.0026775894,0.0008896795,0.028871065],"study_design_scores_gemma":[0.000026227306,0.00008631902,0.95609814,0.0000131231545,0.000030903317,0.00036608466,0.000214332,0.010004567,0.031010184,0.0013844564,0.000745106,0.00002058322],"about_ca_topic_score_codex":0.00076946785,"about_ca_topic_score_gemma":0.0011553257,"teacher_disagreement_score":0.003435398,"about_ca_system_score_codex":0.0002242814,"about_ca_system_score_gemma":0.00009700813,"threshold_uncertainty_score":0.01149255},"labels":[],"label_agreement":null},{"id":"W2091714505","doi":"10.1088/0004-637x/731/2/100","title":"THE ATACAMA COSMOLOGY TELESCOPE: EXTRAGALACTIC SOURCES AT 148 GHz IN THE 2008 SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Sky; Spectral index; Galaxy; Redshift; Telescope; Source counts; Astronomy; Context (archaeology); Cosmology; South Pole Telescope; Radio telescope; Flux (metallurgy); Radio spectrum; Galaxy cluster; Spectral line","score_opus":0.023045174183742727,"score_gpt":0.22982812906669947,"score_spread":0.20678295488295675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091714505","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9253146,0.0007702821,0.0006116249,0.001282178,0.00010257155,0.000046098645,0.05156246,0.00007695225,0.02023326],"genre_scores_gemma":[0.9203261,0.0006134198,0.0016815537,0.0003643674,0.00008268928,0.000075699616,0.05855608,0.000066341265,0.018233705],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982685,0.000029969153,0.0000062033623,0.000035343957,0.000054345273,0.000047379053],"domain_scores_gemma":[0.9994702,0.000049931314,0.00012785148,0.00005786883,0.00015241958,0.00014175398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028407126,0.00011836802,0.0001518292,0.0011671992,0.00041564237,0.00054192974,0.00024500128,0.00029624364,0.0039280513],"category_scores_gemma":[0.0008414861,0.000100394696,0.00008575015,0.0022243538,0.00012255684,0.000542401,0.00077934866,0.000380738,0.00095104985],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002726441,0.00007863736,0.8881851,0.00006458657,0.000044882083,0.00024141248,0.0014644238,0.00018485976,0.002233036,0.0022609513,0.06479033,0.040179092],"study_design_scores_gemma":[0.000008745758,0.0000072914486,0.9665523,0.000011983621,0.0000070652004,0.00006539413,0.00045269233,0.000088430774,0.0001115179,0.00013326238,0.032558084,0.000003212654],"about_ca_topic_score_codex":0.06148504,"about_ca_topic_score_gemma":0.1580413,"teacher_disagreement_score":0.06148504,"about_ca_system_score_codex":0.00046163425,"about_ca_system_score_gemma":0.00056402304,"threshold_uncertainty_score":0.12225431},"labels":[],"label_agreement":null},{"id":"W2091723189","doi":"10.1086/491643","title":"Long‐Term Phase‐coherent X‐Ray Timing of PSR B0540−69","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Glitch; Neutron star; Crab Pulsar; Context (archaeology); Millisecond pulsar; Dipole; Position (finance); Stars","score_opus":0.02267162265391318,"score_gpt":0.3624280336635148,"score_spread":0.3397564110096016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091723189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972253,0.00013218836,0.000946755,0.000017600894,0.0000065155614,0.0000072702073,0.0004664133,0.00004984963,0.0011481127],"genre_scores_gemma":[0.99626166,0.0000825666,0.0015742249,0.000013246989,0.000019600571,0.000010585883,0.0018351685,0.000015317175,0.00018758989],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982774,0.000015635444,0.000012203134,0.00004327348,0.000069115624,0.00003201852],"domain_scores_gemma":[0.99937314,0.000044215063,0.0003342942,0.000053651675,0.00009699067,0.00009770169],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022943802,0.0002758311,0.00019809428,0.0017556429,0.0002784992,0.0003963477,0.00028165572,0.00026756342,0.00053209235],"category_scores_gemma":[0.0008081787,0.00018713767,0.00022869716,0.0010700255,0.00014233004,0.00024605964,0.0004832462,0.00025293828,0.00027004885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057046115,0.00014077898,0.66002816,0.00013410223,0.00018553872,0.0008057875,0.0005930409,0.004717251,0.27050388,0.00123707,0.0009889578,0.060094967],"study_design_scores_gemma":[0.000021093605,0.00014375492,0.9890455,0.000011885753,0.000035077792,0.0005234323,0.00003302584,0.004092748,0.004428071,0.00018326486,0.0014638039,0.0000184875],"about_ca_topic_score_codex":0.0032430089,"about_ca_topic_score_gemma":0.005838153,"teacher_disagreement_score":0.0032430089,"about_ca_system_score_codex":0.00023654164,"about_ca_system_score_gemma":0.00016567757,"threshold_uncertainty_score":0.006448269},"labels":[],"label_agreement":null},{"id":"W2091754923","doi":"10.1088/0004-637x/726/1/23","title":"SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC). II. THE BROWN DWARF POPULATION OF ρ OPHIUCHI","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Brown dwarf; Photometry (optics); Stars; Sky; Population; Extinction (optical mineralogy); Cluster (spacecraft); Star formation","score_opus":0.007117352124993517,"score_gpt":0.2274866235034828,"score_spread":0.2203692713784893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091754923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99920386,0.000112771144,0.000072450544,0.000005473417,0.000002351157,0.0000036669835,0.00009892527,0.000005246318,0.00049510447],"genre_scores_gemma":[0.99885964,0.000077166296,0.00021389363,0.0000061789488,0.0000039091005,0.0000049744135,0.0004776282,0.0000019846077,0.00035461292],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999899,0.000009181221,0.000007941888,0.000025134756,0.000024013414,0.000034705583],"domain_scores_gemma":[0.99958104,0.000035751655,0.00015347054,0.000035507448,0.00005644525,0.0001377577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020067499,0.000115459654,0.00017035723,0.00090464327,0.00060344936,0.00046250262,0.00014159715,0.00009811184,0.0010928196],"category_scores_gemma":[0.00040747426,0.00007771117,0.00011124415,0.000600646,0.0002782086,0.00024466746,0.000833971,0.00012868988,0.00020951442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000085630585,0.000012360585,0.9863413,0.000017318775,0.000012823274,0.00021091144,0.0003906423,0.000050828352,0.007126426,0.00018214225,0.00013091044,0.005438718],"study_design_scores_gemma":[0.0000023547666,0.000029535351,0.99817204,0.0000026459907,0.0000062655477,0.0002374578,0.00027996558,0.00009102267,0.00045296544,0.000034904817,0.0006891929,0.0000016235351],"about_ca_topic_score_codex":0.009930884,"about_ca_topic_score_gemma":0.02175317,"teacher_disagreement_score":0.009930884,"about_ca_system_score_codex":0.0003429848,"about_ca_system_score_gemma":0.0002655433,"threshold_uncertainty_score":0.019746125},"labels":[],"label_agreement":null},{"id":"W2091980209","doi":"10.1086/422160","title":"Light Propagation in Inhomogeneous Universes. IV. Strong Lensing and Environmental Effects","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Dark matter; Strong gravitational lensing; Weak gravitational lensing; Galaxy; Gravitational lensing formalism; Gravitational lens; Redshift; Magnification; Astronomy; Optics","score_opus":0.003585707683854292,"score_gpt":0.17491353592668493,"score_spread":0.17132782824283063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2091980209","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91723067,0.0007173652,0.07430612,0.00022651673,0.000013723999,0.000029731236,0.00022844097,0.00017775332,0.0070696687],"genre_scores_gemma":[0.99235016,0.0003364984,0.006240331,0.000021914471,0.000020514968,0.0000069057633,0.000100071695,0.000020127558,0.000903498],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99957865,0.00016570883,0.000014429326,0.000055532244,0.000084517706,0.00010122238],"domain_scores_gemma":[0.99449867,0.0028083024,0.0012853876,0.0006740453,0.00043986505,0.00029386123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008662352,0.0005187671,0.00024972705,0.0009889276,0.00046032874,0.0008478421,0.0004092724,0.00027509205,0.0015705768],"category_scores_gemma":[0.0058900747,0.0002859737,0.0003374099,0.0009703301,0.0009811472,0.0013490185,0.0008435481,0.00046696735,0.00019073732],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007976165,0.0001356334,0.25961396,0.00035494802,0.00035972107,0.0015518772,0.000537901,0.46346125,0.07472795,0.149724,0.0009394639,0.047795534],"study_design_scores_gemma":[0.0001213895,0.0002828758,0.18222994,0.000040350125,0.0001963711,0.0010356042,0.00041363947,0.674095,0.046827573,0.09097038,0.0036764322,0.00011049847],"about_ca_topic_score_codex":0.004663212,"about_ca_topic_score_gemma":0.004350725,"teacher_disagreement_score":0.004663212,"about_ca_system_score_codex":0.00065904716,"about_ca_system_score_gemma":0.0002465427,"threshold_uncertainty_score":0.009272099},"labels":[],"label_agreement":null},{"id":"W2092053915","doi":"10.1086/497354","title":"Origin of Tidal Dissipation in Jupiter. I. Properties of Inertial Modes","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Inertial wave; Physics; Dissipation; Inertial frame of reference; Jupiter (rocket family); Classical mechanics; Amplitude; Mechanics; Wavelength; Normal mode; Wavenumber; RADIUS; Wave propagation; Quantum mechanics; Vibration; Spacecraft; Longitudinal wave; Mechanical wave","score_opus":0.014731062043356835,"score_gpt":0.2270803912582969,"score_spread":0.21234932921494007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092053915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9553314,0.0017392035,0.02748385,0.00030319102,0.00003131949,0.0000207651,0.000084635554,0.00012151552,0.014884228],"genre_scores_gemma":[0.99726367,0.00021574073,0.001158371,0.000020836107,0.00002128862,0.0000064263727,0.000038523758,0.000020939611,0.0012542421],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999678,0.0000036991692,0.0000018407783,0.000008104299,0.0000066850184,0.000011900673],"domain_scores_gemma":[0.99989617,0.00001821472,0.000039277405,0.0000113318665,0.0000143063235,0.00002060472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010264666,0.00031836657,0.00024081088,0.00033214764,0.0004134897,0.0005605147,0.00030237233,0.00026599178,0.0010794002],"category_scores_gemma":[0.00044857463,0.0001309481,0.00019350187,0.00023900591,0.0005635856,0.00057718746,0.000612695,0.00032106318,0.00016658114],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004222124,0.00012541091,0.17385213,0.00048381186,0.00013025533,0.0033897054,0.0063825506,0.13696046,0.22032526,0.35240406,0.004460658,0.101063594],"study_design_scores_gemma":[0.0000614584,0.0004259304,0.23636971,0.00011151265,0.00009300257,0.0021210592,0.0014554203,0.557829,0.024742723,0.15861207,0.018066354,0.000111805486],"about_ca_topic_score_codex":0.0016991721,"about_ca_topic_score_gemma":0.0010347512,"teacher_disagreement_score":0.0016991721,"about_ca_system_score_codex":0.00041253061,"about_ca_system_score_gemma":0.000100653895,"threshold_uncertainty_score":0.0036109686},"labels":[],"label_agreement":null},{"id":"W2092357828","doi":"10.1086/312556","title":"Cosmic Shear from Galaxy Spins","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":202,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Galaxy; Angular momentum; Gravitational field; Shear (geology); Gravitational lens; Gravitation; Bispectrum; Spins","score_opus":0.010743039742807367,"score_gpt":0.25818651869998055,"score_spread":0.24744347895717317,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092357828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5883099,0.01313862,0.29981953,0.0035124642,0.000732266,0.00006187422,0.0027958576,0.0013385834,0.090290934],"genre_scores_gemma":[0.9742749,0.003909899,0.01417965,0.00014985973,0.000362037,0.000019534687,0.001358563,0.00020971386,0.0055358023],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998745,0.000023318327,0.0000069443495,0.000022233999,0.00005379856,0.000019318322],"domain_scores_gemma":[0.99928635,0.00035746687,0.00014157593,0.00009816428,0.00007056893,0.000046044883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044275878,0.0005896931,0.00038654014,0.0011552045,0.00031031866,0.0012805344,0.00031005635,0.0004018988,0.004956405],"category_scores_gemma":[0.005367312,0.00027871117,0.00038771852,0.0011553433,0.0006766385,0.0012090828,0.0013105083,0.00067434116,0.0010378071],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018592483,0.000028772922,0.050217688,0.0004775054,0.00018359486,0.00037276998,0.0004192143,0.3717266,0.0145181455,0.39689302,0.0048124525,0.16016434],"study_design_scores_gemma":[0.000021235257,0.0000809186,0.074898645,0.0002354337,0.00008151298,0.0005974798,0.00013636387,0.46211383,0.010840544,0.4282716,0.022529963,0.00019251253],"about_ca_topic_score_codex":0.004326635,"about_ca_topic_score_gemma":0.002488238,"teacher_disagreement_score":0.004956405,"about_ca_system_score_codex":0.000645199,"about_ca_system_score_gemma":0.00029222522,"threshold_uncertainty_score":0.01658082},"labels":[],"label_agreement":null},{"id":"W2092378236","doi":"10.1088/0004-637x/742/2/127","title":"MULTIWAVELENGTH OBSERVATIONS OF THE PREVIOUSLY UNIDENTIFIED BLAZAR RX J0648.7+1516","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Blazar; Astrophysics; Astronomy; Quasar; Galaxy; Gamma ray","score_opus":0.03063154686015312,"score_gpt":0.21847368590211022,"score_spread":0.1878421390419571,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092378236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99795854,0.00019538554,0.00011776409,0.000039001898,0.000013051846,0.000006096956,0.00040921848,0.000033804616,0.0012269989],"genre_scores_gemma":[0.99583554,0.00015481937,0.0010106834,0.00007142656,0.00005853354,0.000009603225,0.001864204,0.0000126233235,0.0009826424],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997893,0.0000138838,0.000009831831,0.00007078473,0.000071522874,0.000044712015],"domain_scores_gemma":[0.99961287,0.000027010592,0.00016489883,0.000070259666,0.00003479705,0.000090183545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024523173,0.00024870838,0.0002932825,0.00067632226,0.00043980355,0.00044149315,0.00046249776,0.00043656406,0.0012914533],"category_scores_gemma":[0.00032983968,0.00019973521,0.00019699804,0.00035524485,0.00025322035,0.00025699518,0.0004520766,0.00042981975,0.0006860819],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008247892,0.00036162243,0.6217379,0.00016556353,0.00020362408,0.0045526805,0.0008190554,0.0006346341,0.33365816,0.000604496,0.0030428336,0.033394698],"study_design_scores_gemma":[0.00003995364,0.00031339808,0.9856903,0.000014959671,0.000033497163,0.0022889115,0.0001118483,0.0004956309,0.0055781403,0.00007704072,0.005341822,0.000014502979],"about_ca_topic_score_codex":0.0012030688,"about_ca_topic_score_gemma":0.0047029187,"teacher_disagreement_score":0.0012914533,"about_ca_system_score_codex":0.00021442458,"about_ca_system_score_gemma":0.00012150619,"threshold_uncertainty_score":0.0043203235},"labels":[],"label_agreement":null},{"id":"W2092456387","doi":"10.1086/317884","title":"A Deep Submillimeter Survey of the Galactic Center","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":199,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Galactic Center; James Clerk Maxwell Telescope; Galactic plane; Astrophysics; Astronomy; Molecular cloud; Submillimeter Array; Bolometer; Telescope; Galaxy; Star formation; Stars","score_opus":0.012742947992907304,"score_gpt":0.23189122311602292,"score_spread":0.2191482751231156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092456387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98014647,0.0014035295,0.00095502957,0.0003699926,0.000030832613,0.000037975755,0.0063370876,0.00012052154,0.010598505],"genre_scores_gemma":[0.982752,0.0007880357,0.0031356046,0.00029713492,0.00007314378,0.000023698234,0.0099275345,0.000031904856,0.0029710615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992514,0.0000068498384,0.0000025284794,0.000021919106,0.00002301576,0.000020576117],"domain_scores_gemma":[0.99979967,0.0000084848925,0.000039157676,0.000024519932,0.000042661726,0.00008548745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011219001,0.00017885206,0.00012275942,0.0010537816,0.00026018865,0.00032998092,0.00016649332,0.00017680903,0.0012774738],"category_scores_gemma":[0.00022330393,0.00008465009,0.000074581476,0.0009413962,0.00010478401,0.0002767784,0.00048609945,0.00022955441,0.00043480287],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000110977875,0.00012340774,0.80585283,0.000109982415,0.00012345106,0.00029639102,0.0010934618,0.00048454007,0.03771285,0.0013566408,0.013609515,0.13912587],"study_design_scores_gemma":[0.000006365179,0.000021822028,0.9809905,0.00000829788,0.000008373105,0.00007182228,0.00012984451,0.00017820587,0.00047989565,0.00012410711,0.017977893,0.0000028650932],"about_ca_topic_score_codex":0.016848523,"about_ca_topic_score_gemma":0.040300556,"teacher_disagreement_score":0.016848523,"about_ca_system_score_codex":0.00030841038,"about_ca_system_score_gemma":0.00030570372,"threshold_uncertainty_score":0.03350091},"labels":[],"label_agreement":null},{"id":"W2092545093","doi":"10.1086/521541","title":"The Masses and Shapes of Dark Matter Halos from Galaxy‐Galaxy Lensing in the CFHT Legacy Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Victoria; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Dark galaxy; Dark matter; Galaxy; Dark matter halo; Halo; Astronomy; Galaxy group; Virial mass; Redshift; Velocity dispersion; Galaxy formation and evolution","score_opus":0.011655755849863713,"score_gpt":0.22918484720335877,"score_spread":0.21752909135349505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092545093","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962347,0.000278387,0.00006171837,0.00010097703,0.0000038899993,0.0000024077408,0.0021176336,0.000015292648,0.0011849857],"genre_scores_gemma":[0.99832314,0.00010617853,0.000038142083,0.000017647077,0.000011543165,9.537816e-7,0.0012329218,0.000004168117,0.00026524704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998957,0.000013204481,0.0000060721636,0.000026221756,0.000021326352,0.00003741853],"domain_scores_gemma":[0.99837697,0.00030282504,0.0006174894,0.00012419905,0.00022684355,0.00035174278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062205887,0.0002052146,0.00020673487,0.0019630697,0.0003588736,0.00066814973,0.00023750369,0.00031055158,0.0026906647],"category_scores_gemma":[0.002299165,0.00020077986,0.00026646745,0.0011661747,0.00029811644,0.00051183987,0.00072592386,0.00023498923,0.0003599044],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008348233,0.000004648949,0.99322563,0.000010482125,0.000035385274,0.000047071622,0.000254057,0.00020030362,0.001104146,0.00022035123,0.00071046315,0.0041040317],"study_design_scores_gemma":[0.0000010078875,0.0000026454306,0.9996487,0.0000015497764,0.000004820631,0.000025196134,0.000050872404,0.000057733738,0.000043414573,0.00004192855,0.000120624674,0.0000015961682],"about_ca_topic_score_codex":0.029243406,"about_ca_topic_score_gemma":0.06033482,"teacher_disagreement_score":0.029243406,"about_ca_system_score_codex":0.0005975956,"about_ca_system_score_gemma":0.00022358386,"threshold_uncertainty_score":0.058146417},"labels":[],"label_agreement":null},{"id":"W2092550005","doi":"10.1086/432245","title":"High‐Energy Emission from Magnetars","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Pulsar; Bremsstrahlung; Magnetar; Astrophysics; Electron; Magnetosphere; Soft photon; Luminosity; Photon; Gamma ray; Atomic physics; Plasma; Nuclear physics; Galaxy; Optics","score_opus":0.007803568155514635,"score_gpt":0.27672653842028244,"score_spread":0.2689229702647678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092550005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99579227,0.0006893202,0.00056694256,0.000050834577,0.000007968011,0.0000035415983,0.00006032462,0.000052767224,0.0027760467],"genre_scores_gemma":[0.99820006,0.00026905682,0.0003974624,0.0000298239,0.000016915068,0.0000040717136,0.00012406566,0.000010374603,0.00094814424],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999521,0.0000050307476,0.000001506778,0.00001396512,0.000009898277,0.000017431463],"domain_scores_gemma":[0.999941,0.000014635437,0.000018449582,0.0000069408716,0.000007576244,0.000011315409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008795861,0.00022633141,0.0001580082,0.0003688007,0.00023844758,0.00046856364,0.0001856694,0.00028553617,0.0014755805],"category_scores_gemma":[0.000114815404,0.00016926513,0.00015738809,0.00023514747,0.00017174293,0.00012684645,0.0003622216,0.00019933569,0.00035141633],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031854457,0.000040515282,0.043619536,0.00014437472,0.000054304597,0.0011940007,0.00028970616,0.00045492538,0.93617666,0.0012251842,0.0006911723,0.015791109],"study_design_scores_gemma":[0.000083824416,0.0004363339,0.7564101,0.000036438014,0.00009587174,0.004036072,0.0003236758,0.002200502,0.22407335,0.0009009658,0.011361873,0.000040976454],"about_ca_topic_score_codex":0.0002862645,"about_ca_topic_score_gemma":0.0003522809,"teacher_disagreement_score":0.0014755805,"about_ca_system_score_codex":0.00022679067,"about_ca_system_score_gemma":0.000043854063,"threshold_uncertainty_score":0.004936278},"labels":[],"label_agreement":null},{"id":"W2092753569","doi":"10.1088/0004-637x/751/1/28","title":"EVIDENCE FOR ENVIRONMENTAL CHANGES IN THE SUBMILLIMETER DUST OPACITY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Opacity; Physics; Emissivity; Astrophysics; Galactic plane; Cosmic dust; Radiance; Interstellar medium; Black-body radiation; Molecular cloud; Extinction (optical mineralogy); Astronomy; Stars; Galaxy; Optics; Radiation","score_opus":0.05215039318998442,"score_gpt":0.2774893872258678,"score_spread":0.22533899403588337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092753569","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99859124,0.000069485686,0.000112995695,0.00002309981,0.0000019996814,0.000002235325,0.00026370687,0.000010660906,0.00092459493],"genre_scores_gemma":[0.999241,0.000037331283,0.00010690579,0.000021788415,0.000004398144,0.00000308366,0.00024206398,0.000006339636,0.00033706485],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998815,0.000015921922,0.0000073913147,0.0000452155,0.000019319765,0.000030657073],"domain_scores_gemma":[0.99918145,0.00012343844,0.0003601159,0.000079245234,0.00012669656,0.00012910158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015439533,0.00015840509,0.00018348027,0.0004366781,0.00026150254,0.0005044636,0.00024953758,0.00036954944,0.0016963353],"category_scores_gemma":[0.00061481755,0.00018605663,0.00016646077,0.0005253682,0.00036548008,0.00032813847,0.000326339,0.00027833306,0.0003364357],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001563981,0.000054193173,0.9547042,0.000016520893,0.000048546124,0.00021522222,0.00020353796,0.00012535269,0.040653862,0.00010767059,0.000096314114,0.0036182988],"study_design_scores_gemma":[5.936905e-7,0.000009875564,0.999423,5.76665e-7,0.0000020053956,0.000043789652,0.00003302429,0.00002834551,0.000354112,0.0000073415627,0.00009644548,9.1160297e-7],"about_ca_topic_score_codex":0.002518847,"about_ca_topic_score_gemma":0.004965658,"teacher_disagreement_score":0.002518847,"about_ca_system_score_codex":0.0002156708,"about_ca_system_score_gemma":0.000087874774,"threshold_uncertainty_score":0.005674839},"labels":[],"label_agreement":null},{"id":"W2092753575","doi":"10.1088/0004-637x/775/1/52","title":"LIMITS ON THE NUMBER OF GALACTIC YOUNG SUPERNOVA REMNANTS EMITTING IN THE DECAY LINES OF<sup>44</sup>Ti","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Supernova; Physics; Astrophysics; Galaxy; Flux (metallurgy); Decay chain; Photon; Near-Earth supernova; Astronomy; Supernova remnant; Nuclear physics","score_opus":0.01795092870571652,"score_gpt":0.2527088258664215,"score_spread":0.234757897160705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092753575","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8782853,0.0018729485,0.10822391,0.00047740721,0.00002912386,0.00004726809,0.0012298828,0.0004922185,0.009342024],"genre_scores_gemma":[0.99223363,0.00030623746,0.0065667527,0.00005286741,0.000028513765,0.000018602168,0.00057070237,0.000018982833,0.00020373952],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.998755,0.0004172864,0.00015312027,0.0002528338,0.00027948464,0.0001423751],"domain_scores_gemma":[0.96466756,0.025523994,0.005121371,0.0024481453,0.0015248662,0.00071408745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005305643,0.0009276515,0.0005924682,0.0011029909,0.0004425059,0.0015795383,0.0017981046,0.0011429252,0.0026680124],"category_scores_gemma":[0.026029307,0.0005497173,0.0010844433,0.0005122454,0.001361647,0.0019176488,0.0010294326,0.00067067833,0.0005959163],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010078159,0.00008141221,0.7810991,0.00027263394,0.00035849088,0.0007109339,0.00025483264,0.14119536,0.01471837,0.027404584,0.0009901442,0.031906378],"study_design_scores_gemma":[0.000087340275,0.00075855886,0.3245154,0.000379711,0.0003069207,0.0035270024,0.00044846282,0.5736543,0.034677472,0.05565761,0.0058093844,0.00017783346],"about_ca_topic_score_codex":0.0019055124,"about_ca_topic_score_gemma":0.001629657,"teacher_disagreement_score":0.005305643,"about_ca_system_score_codex":0.0007245371,"about_ca_system_score_gemma":0.0003015389,"threshold_uncertainty_score":0.028059304},"labels":[],"label_agreement":null},{"id":"W2092823919","doi":"10.1088/0004-637x/773/2/173","title":"A GALACTIC WEIGH-IN: MASS MODELS OF SINGS GALAXIES USING CHEMO-SPECTROPHOTOMETRIC GALACTIC EVOLUTION MODELS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astrophysics; Physics; Bulge; Galaxy; Spiral galaxy; Disc; Stellar population; Galaxy formation and evolution; Halo; Stellar mass; Photometry (optics); Astronomy; Dark matter halo; Population; Dark matter; Thick disk; Star formation; Stars","score_opus":0.014198626546976775,"score_gpt":0.21641025552883336,"score_spread":0.20221162898185657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092823919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.66297233,0.0023495655,0.2515081,0.009041423,0.0003896136,0.0001210651,0.0012344636,0.0014063708,0.07097705],"genre_scores_gemma":[0.9756782,0.0003940064,0.0076889573,0.0004200509,0.00025951467,0.000046691464,0.00026018824,0.0003391358,0.014913309],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999021,0.00004491199,0.00000365124,0.000017997902,0.000012982168,0.000018287777],"domain_scores_gemma":[0.9992111,0.00034688023,0.00011719686,0.0000674185,0.00008119778,0.0001762092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00079973944,0.0008882636,0.0008976827,0.0005877844,0.0010571138,0.0018739759,0.002543014,0.0018901186,0.0050672027],"category_scores_gemma":[0.0034025756,0.00074275525,0.0012779916,0.00047847556,0.00080506847,0.0023588839,0.0013000706,0.0011399372,0.0009824436],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000092918286,0.000061342485,0.009101305,0.000052112548,0.000103899736,0.00025879554,0.00022010639,0.8264231,0.0012219105,0.14829029,0.0051421127,0.009032042],"study_design_scores_gemma":[0.00002070064,0.000007445872,0.00073765975,0.0000064651877,0.000017537068,0.000028342816,0.000022147335,0.97786885,0.000117336065,0.020560617,0.0006014001,0.000011431979],"about_ca_topic_score_codex":0.023433695,"about_ca_topic_score_gemma":0.0136380475,"teacher_disagreement_score":0.023433695,"about_ca_system_score_codex":0.0012912651,"about_ca_system_score_gemma":0.0005090774,"threshold_uncertainty_score":0.04659456},"labels":[],"label_agreement":null},{"id":"W2092886761","doi":"10.1088/0004-637x/757/1/64","title":"STAR FORMATION IN THE OUTER DISK OF SPIRAL GALAXIES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Star formation; Spiral galaxy; RADIUS; Thick disk; Astronomy; Galaxy; Thin disk; Gravitational collapse; Debris disk; Star (game theory); Accretion (finance); Stars; Planetary system","score_opus":0.010782978700961022,"score_gpt":0.2204875571479667,"score_spread":0.20970457844700569,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092886761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996897,0.000059144073,0.00006762754,0.0000026192474,3.2993592e-7,9.3338724e-7,0.000039160277,0.0000040949444,0.0001364235],"genre_scores_gemma":[0.9996271,0.000040569823,0.0001347541,0.0000035047913,0.0000016287078,0.0000010177022,0.00013618192,0.0000013760267,0.000053751206],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985266,0.000014744927,0.000010283561,0.00005813302,0.000031832948,0.000032377782],"domain_scores_gemma":[0.99906904,0.00011488601,0.00042768742,0.000091580616,0.00011564096,0.00018114071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026553948,0.00021067746,0.00024071286,0.0013850393,0.00019149885,0.0006126723,0.00019167805,0.00013580227,0.00027940026],"category_scores_gemma":[0.0009098489,0.00017428107,0.00016582834,0.0005855017,0.00037251392,0.00031099154,0.00044991844,0.00010876065,0.00010213609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000955374,0.000009930107,0.9786236,0.0000116139345,0.00004222097,0.00007826001,0.00030821297,0.00037502663,0.015931915,0.000042776628,0.000031746902,0.0044490756],"study_design_scores_gemma":[0.0000027035605,0.000027848475,0.9984763,0.0000026686482,0.000012276049,0.00008974274,0.00007259768,0.0004938445,0.00064859714,0.000037240974,0.00013314468,0.000002996544],"about_ca_topic_score_codex":0.0068669994,"about_ca_topic_score_gemma":0.009138945,"teacher_disagreement_score":0.0068669994,"about_ca_system_score_codex":0.0004972531,"about_ca_system_score_gemma":0.0001318153,"threshold_uncertainty_score":0.013654053},"labels":[],"label_agreement":null},{"id":"W2092887956","doi":"10.1088/0004-637x/745/1/31","title":"THE<i>HUBBLE SPACE TELESCOPE</i>CLUSTER SUPERNOVA SURVEY. VI. THE VOLUMETRIC TYPE Ia SUPERNOVA RATE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Supernova; Physics; Astrophysics; Redshift; Hubble space telescope; Galaxy; Flattening; Extinction (optical mineralogy); Cluster (spacecraft); Redshift survey; Astronomy; Advanced Camera for Surveys; Hubble's law; Type (biology); Optics","score_opus":0.023086241223672088,"score_gpt":0.23962832454343314,"score_spread":0.21654208331976105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2092887956","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5390382,0.0049987193,0.007005311,0.00085168163,0.00033644546,0.00045099025,0.38800913,0.0018052898,0.05750424],"genre_scores_gemma":[0.735051,0.0034953991,0.0121952165,0.00037316605,0.00031652773,0.0002446443,0.23060204,0.00021015672,0.017511884],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997645,0.000031415926,0.00001692746,0.00004035493,0.000097917495,0.000048827376],"domain_scores_gemma":[0.99844176,0.00008533252,0.0005887534,0.00014131684,0.00030823488,0.00043453602],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006629978,0.0005124784,0.0002534307,0.004770511,0.00024805643,0.0004171358,0.0003857268,0.00023930895,0.0029628896],"category_scores_gemma":[0.0010873663,0.00012550352,0.0002768705,0.0029928433,0.00015218054,0.00032506,0.00054727943,0.00031728274,0.0017305936],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029166482,0.000077175544,0.82578856,0.0002700456,0.00034682674,0.00019157009,0.00022090814,0.0013244494,0.005481153,0.0023044583,0.085425116,0.0782781],"study_design_scores_gemma":[0.000014418504,0.000040303712,0.9654208,0.000027617642,0.000030851636,0.00011020173,0.000028343848,0.0004019961,0.00070237386,0.00026805248,0.032945834,0.00000928214],"about_ca_topic_score_codex":0.035231017,"about_ca_topic_score_gemma":0.056499463,"teacher_disagreement_score":0.035231017,"about_ca_system_score_codex":0.0007852172,"about_ca_system_score_gemma":0.00042198622,"threshold_uncertainty_score":0.07005191},"labels":[],"label_agreement":null},{"id":"W2093077071","doi":"10.1086/320638","title":"Final Results from the<i>Hubble Space Telescope</i>Key Project to Measure the Hubble Constant","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3311,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Hubble's law; Distance modulus; Galaxy; Spiral galaxy; Hubble space telescope; Cosmic distance ladder; Advanced Camera for Surveys; Hubble Ultra-Deep Field","score_opus":0.02063981775847328,"score_gpt":0.23162261864681447,"score_spread":0.21098280088834118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093077071","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0894292,0.0145705035,0.33386213,0.0057074563,0.0035476745,0.0024329748,0.33911932,0.009490182,0.20184056],"genre_scores_gemma":[0.18326914,0.005285779,0.37519842,0.0025477016,0.0010718064,0.0029744941,0.35251674,0.004501513,0.072634414],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99172103,0.0014189166,0.000287392,0.00097384653,0.0048237825,0.00077502587],"domain_scores_gemma":[0.9851613,0.00090855674,0.0007429928,0.0027533204,0.008954755,0.0014790514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.011506962,0.002539463,0.0012938892,0.0041652573,0.0010535266,0.0041865697,0.00166837,0.0012137636,0.012132313],"category_scores_gemma":[0.00860848,0.000754685,0.0018288367,0.0027148123,0.0006284901,0.0017408526,0.0029677094,0.0017508684,0.015507244],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025760198,0.00063554524,0.081185676,0.0012924629,0.0011050832,0.00019237265,0.00055013865,0.011276801,0.034595873,0.02180368,0.44423637,0.40054995],"study_design_scores_gemma":[0.00024085281,0.0007990167,0.2566172,0.0003107048,0.0007437711,0.00032700782,0.00031375542,0.006244486,0.059315473,0.009513517,0.66528344,0.0002908343],"about_ca_topic_score_codex":0.01286944,"about_ca_topic_score_gemma":0.010339618,"teacher_disagreement_score":0.01286944,"about_ca_system_score_codex":0.00264256,"about_ca_system_score_gemma":0.0027216983,"threshold_uncertainty_score":0.06085533},"labels":[],"label_agreement":null},{"id":"W2093089525","doi":"10.1086/505740","title":"The Infrared Counterpart to the Magnetar 1RXS J170849.0−400910","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Magnetar; Pulsar; Infrared; Physics; Astrophysics; Object (grammar); Flux (metallurgy); Neutron star; Position (finance); Astronomy; Field (mathematics); Star (game theory); Computer science; Mathematics; Materials science; Artificial intelligence; Pure mathematics","score_opus":0.006048018009891229,"score_gpt":0.2796355225470926,"score_spread":0.2735875045372014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093089525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975055,0.000111086774,0.00021795249,0.00003997145,0.000008639957,0.0000024135932,0.00023087165,0.000017198328,0.0018664034],"genre_scores_gemma":[0.9951375,0.00011258545,0.0013697827,0.00004976187,0.00005353424,0.0000062089052,0.0016552085,0.000014470293,0.0016010641],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989617,0.0000073461943,0.0000046611967,0.00003481096,0.000030691866,0.000026394282],"domain_scores_gemma":[0.9996209,0.000043318327,0.0001733419,0.000042631083,0.0000628756,0.000056792975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002553239,0.00013180196,0.00018485734,0.0009633216,0.00042564777,0.0004303903,0.00023000441,0.00017093666,0.0015322566],"category_scores_gemma":[0.00043675012,0.00009394717,0.00009987783,0.00067094207,0.00022829567,0.00031774378,0.00053033204,0.00023532577,0.0003989487],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048477674,0.0001832931,0.77250254,0.00014795137,0.00009283263,0.0020657224,0.0010440341,0.00057815725,0.1713289,0.0027513625,0.0021903852,0.046630062],"study_design_scores_gemma":[0.000016496244,0.000073368916,0.98612577,0.000010018253,0.000035832873,0.00094947574,0.00024107937,0.0005358085,0.004340118,0.00047974222,0.007184932,0.0000072608636],"about_ca_topic_score_codex":0.00091632595,"about_ca_topic_score_gemma":0.0022432255,"teacher_disagreement_score":0.0015322566,"about_ca_system_score_codex":0.00016762318,"about_ca_system_score_gemma":0.00014148756,"threshold_uncertainty_score":0.0051258802},"labels":[],"label_agreement":null},{"id":"W2093148048","doi":"10.1086/308157","title":"Simultaneous X‐Ray and Radio Monitoring of the Unusual Binary LS I +61o303: Measurements of the Light Curve and High‐Energy Spectrum","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Office of Naval Research; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Quasar; Light curve; Pulsar; Gamma ray; Compton scattering; Redshift; Photon; Flux (metallurgy); Astronomy; Galaxy; Optics","score_opus":0.011924355678740733,"score_gpt":0.21401512898307792,"score_spread":0.2020907733043372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093148048","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992131,0.00004708932,0.000084061154,0.000010078641,0.0000013105889,0.0000036536894,0.000098783734,0.0000059193358,0.0005360041],"genre_scores_gemma":[0.99906546,0.000051608422,0.00025471865,0.00001728654,0.000007351398,0.0000054082607,0.0004018695,0.000005133253,0.00019118542],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998938,0.000011604296,0.000008796064,0.00002605673,0.000031364933,0.00002841796],"domain_scores_gemma":[0.9996259,0.0000331239,0.00013933265,0.000033817785,0.00004746087,0.000120399774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001982685,0.00019011689,0.00026979562,0.0005029984,0.00037174995,0.0005409528,0.00016763741,0.00028500173,0.0006762961],"category_scores_gemma":[0.00038266127,0.00019827984,0.000103817576,0.0005109997,0.00028281062,0.00025623254,0.0004927527,0.00037045495,0.00028828578],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048109863,0.00013846808,0.7098132,0.00006107311,0.00004697398,0.00090743235,0.00053557556,0.00030314294,0.2772504,0.00023655269,0.00032081958,0.009905419],"study_design_scores_gemma":[0.000010718163,0.00013237695,0.99553573,0.0000041491803,0.000013694391,0.00059628434,0.00010940546,0.0002497428,0.0029287818,0.00004448215,0.00036922796,0.000005455113],"about_ca_topic_score_codex":0.0018560463,"about_ca_topic_score_gemma":0.006042379,"teacher_disagreement_score":0.0018560463,"about_ca_system_score_codex":0.00018164709,"about_ca_system_score_gemma":0.00015845934,"threshold_uncertainty_score":0.0036904812},"labels":[],"label_agreement":null},{"id":"W2093303317","doi":"10.1086/426668","title":"Studies of the Relativistic Binary Pulsar PSR B1534+12. II. Origin and Evolution","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Neutron star; Astrophysics; Roche lobe; Pulsar; Supernova; X-ray pulsar; Astronomy; X-ray binary; Binary star; Helium; X-ray burster; Binary pulsar; Stellar evolution; Millisecond pulsar; Stellar mass loss; Stars; Atomic physics","score_opus":0.022751160278981875,"score_gpt":0.3375207496087501,"score_spread":0.31476958932976823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093303317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747074,0.0011414259,0.00040781862,0.00004441242,0.000010630434,0.0000045068277,0.000049158476,0.000010791066,0.00086063833],"genre_scores_gemma":[0.9963553,0.00092426914,0.0015062015,0.00004731497,0.00001491142,0.000008558304,0.0004360741,0.0000082135275,0.0006991329],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990344,0.000012879155,0.000010165094,0.000027781487,0.00002432148,0.000021413254],"domain_scores_gemma":[0.99963284,0.000027485099,0.0002187206,0.00002478721,0.00004925216,0.000046956327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034076785,0.00022643048,0.000278276,0.000797919,0.00060931133,0.0005438918,0.00026707508,0.00028151477,0.00036344834],"category_scores_gemma":[0.0006387776,0.00021988123,0.00016692361,0.00079177675,0.0002868404,0.00021723207,0.00047127274,0.00032593016,0.0001990918],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000528217,0.00012964578,0.48649693,0.00023754209,0.000118100805,0.0011352083,0.0010119564,0.0008267974,0.45756122,0.0033662743,0.00035584538,0.048232336],"study_design_scores_gemma":[0.000026946254,0.0005187158,0.93689215,0.000033795306,0.00009602995,0.0028682307,0.00044451572,0.0020264531,0.041930478,0.0006991176,0.014438031,0.000025555571],"about_ca_topic_score_codex":0.00434392,"about_ca_topic_score_gemma":0.00408748,"teacher_disagreement_score":0.00434392,"about_ca_system_score_codex":0.00062390306,"about_ca_system_score_gemma":0.00023274496,"threshold_uncertainty_score":0.008637309},"labels":[],"label_agreement":null},{"id":"W2093315232","doi":"10.1088/0004-637x/736/1/28","title":"A POPULATION OF X-RAY WEAK QUASARS: PHL 1811 ANALOGS AT HIGH REDSHIFT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Redshift; Population; Sky; Brightness; Emission spectrum; Spectral energy distribution; Spectral line","score_opus":0.012386108219604008,"score_gpt":0.2108600308663818,"score_spread":0.1984739226467778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093315232","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995128,0.000055063465,0.000048716625,0.000012081462,0.0000012156951,0.000004456286,0.00009047937,0.0000034348268,0.00027177445],"genre_scores_gemma":[0.99931896,0.00004496304,0.000059304366,0.000027385851,0.000008023271,0.000003489592,0.00027176892,0.0000044182384,0.00026174824],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997272,0.000026644759,0.000021014854,0.00010177701,0.00005394753,0.00006939192],"domain_scores_gemma":[0.99897885,0.00007846991,0.00042268872,0.000099485056,0.00009691089,0.0003236978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028651653,0.00035666823,0.00048156639,0.0015721539,0.0008227674,0.0012576747,0.00045508548,0.00027600286,0.0019230228],"category_scores_gemma":[0.00067146437,0.00022317408,0.00017180743,0.00074312015,0.00072232576,0.0005323891,0.0010204536,0.00042955147,0.0007877846],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003177966,0.00014862433,0.97819626,0.000013090203,0.000037726197,0.0004176059,0.0008408254,0.0000404218,0.015744802,0.00014615653,0.00011172649,0.0039848597],"study_design_scores_gemma":[0.0000127694275,0.00019908033,0.99567103,0.0000025000693,0.00001856963,0.0019792414,0.00085451064,0.00007613875,0.00066813926,0.000071737435,0.0004386006,0.000007751878],"about_ca_topic_score_codex":0.0015383821,"about_ca_topic_score_gemma":0.001974122,"teacher_disagreement_score":0.0019230228,"about_ca_system_score_codex":0.00019018125,"about_ca_system_score_gemma":0.00013984166,"threshold_uncertainty_score":0.0064331293},"labels":[],"label_agreement":null},{"id":"W2093410738","doi":"10.1086/339843","title":"Australia Telescope Compact Array Radio Imaging of the Proplyd‐like Objects in the Giant H<scp>ii</scp>Region NGC 3603","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Telescope; Radio telescope; X-shaped radio galaxy; Basso continuo; Spectral line; H II region; Giant Metrewave Radio Telescope; Luminosity","score_opus":0.021052182029673197,"score_gpt":0.23983566141028878,"score_spread":0.2187834793806156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093410738","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959293,0.00015838227,0.00035070378,0.000058177517,0.000005086104,0.000014008833,0.00039341798,0.000044634297,0.003046192],"genre_scores_gemma":[0.9964812,0.00010859831,0.0017643225,0.000049468454,0.000012011725,0.000010405904,0.0004866389,0.000009432509,0.0010779236],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991906,0.0000046019036,0.0000047345316,0.000023904811,0.00003244067,0.000015244143],"domain_scores_gemma":[0.9997367,0.000017161674,0.00007427215,0.000029118028,0.000044752785,0.00009792589],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013771896,0.00011785467,0.00011782591,0.0011081336,0.0002746125,0.0003213048,0.0002384062,0.00024253997,0.0014256183],"category_scores_gemma":[0.00018204139,0.00019470655,0.00014085944,0.0006881426,0.0001947669,0.00015566795,0.0004195065,0.00023232793,0.00038103375],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005526841,0.000111369525,0.3207054,0.000113133465,0.0000860656,0.001963974,0.0014174503,0.0005067917,0.640192,0.0005000617,0.0025391232,0.031311885],"study_design_scores_gemma":[0.000009247958,0.00004699417,0.99618834,0.000004225947,0.000008733431,0.00078266754,0.00009222227,0.00025596636,0.0016497434,0.00003750173,0.0009202407,0.000004090132],"about_ca_topic_score_codex":0.00662787,"about_ca_topic_score_gemma":0.013993248,"teacher_disagreement_score":0.00662787,"about_ca_system_score_codex":0.00022826451,"about_ca_system_score_gemma":0.000108678236,"threshold_uncertainty_score":0.013178587},"labels":[],"label_agreement":null},{"id":"W2093462453","doi":"10.1088/0004-637x/769/2/118","title":"THE<i>H</i>-BAND EMITTING REGION OF THE LUMINOUS BLUE VARIABLE P CYGNI: SPECTROPHOTOMETRY AND INTERFEROMETRY OF THE WIND","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"College of Arts and Sciences, Boston University; Science and Technology Facilities Council; NASA Exoplanet Science Institute; National Aeronautics and Space Administration; Georgia State University; Louisiana Board of Regents; W. M. Keck Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Flux (metallurgy); Photosphere; Luminous blue variable; Interferometry; Astronomy; Angular resolution (graph drawing); Halo; Spectral energy distribution; Telescope; Galaxy; Spectral line; Stars","score_opus":0.0061851572137798655,"score_gpt":0.19209548986106506,"score_spread":0.18591033264728518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093462453","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99474925,0.000749174,0.0006951813,0.0001961135,0.00002715447,0.000006453549,0.0001477013,0.00006047952,0.0033684934],"genre_scores_gemma":[0.9981774,0.00028290143,0.00044017308,0.000026713918,0.000044355733,0.0000030188858,0.00015752428,0.000024193168,0.00084367197],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994206,0.0000068140153,0.0000014681466,0.00001709456,0.000021440545,0.00001114185],"domain_scores_gemma":[0.99979204,0.00003197798,0.00007894551,0.0000136274475,0.000045162502,0.000038353377],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021677895,0.00019772837,0.0001413492,0.000986823,0.000330165,0.0005629768,0.00027945836,0.00026630185,0.0013013596],"category_scores_gemma":[0.0006293878,0.00019681535,0.00006245548,0.0006087303,0.00027359382,0.00044702663,0.0003034958,0.0002529959,0.00031431508],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037385532,0.00007709571,0.57564056,0.00016953595,0.00011630009,0.0009052072,0.0008899655,0.0014571386,0.34005913,0.0034029188,0.006011113,0.07089721],"study_design_scores_gemma":[0.000014472413,0.000022953047,0.98731005,0.000010501928,0.000024994975,0.00022673729,0.0000921275,0.0013522856,0.0070670336,0.00036551812,0.0035060756,0.0000072198795],"about_ca_topic_score_codex":0.0030127629,"about_ca_topic_score_gemma":0.0068318676,"teacher_disagreement_score":0.0030127629,"about_ca_system_score_codex":0.00025699934,"about_ca_system_score_gemma":0.00022022934,"threshold_uncertainty_score":0.005990505},"labels":[],"label_agreement":null},{"id":"W2093502522","doi":"10.1086/591835","title":"The Very Low Albedo of an Extrasolar Planet:<i>MOST</i>Space‐based Photometry of HD 209458","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":211,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Saint Mary's University; St. Mary's University; University of British Columbia","funders":"","keywords":"Geometric albedo; Exoplanet; Physics; Photometry (optics); Hot Jupiter; Planet; Astrophysics; Spitzer Space Telescope; Astronomy; Light curve; Albedo (alchemy); Planetary system; Eclipse; Stars","score_opus":0.010495795712461557,"score_gpt":0.220667029677566,"score_spread":0.21017123396510443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093502522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927856,0.00016634558,0.0023993775,0.00006442814,0.000009848692,0.000009122147,0.0007297091,0.00016086643,0.0036748128],"genre_scores_gemma":[0.99829274,0.0000325098,0.0009391234,0.000023494782,0.0000052775486,0.000005965612,0.0005125838,0.000023755798,0.00016459721],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998734,0.000012304509,0.0000067825063,0.000051960276,0.00002779626,0.000027800186],"domain_scores_gemma":[0.9998447,0.000024973499,0.000046390167,0.000028827008,0.000022398699,0.000032678552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014664102,0.0002981574,0.00016712683,0.0006617567,0.0004107616,0.0005113152,0.00031882647,0.00029492532,0.0013167904],"category_scores_gemma":[0.00039155324,0.00017384524,0.00024113,0.00044651836,0.00024265285,0.00024615164,0.00039299374,0.00028083895,0.0003814521],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016711636,0.00006256557,0.7838237,0.00012191331,0.00012534487,0.00031404145,0.00030189147,0.0063555078,0.1854904,0.0017805459,0.002397184,0.019059697],"study_design_scores_gemma":[0.000019470004,0.000039534272,0.9750196,0.000009480963,0.00002912096,0.00020922888,0.000072148236,0.0072263516,0.014047258,0.00026445955,0.0030506225,0.000012806533],"about_ca_topic_score_codex":0.008090175,"about_ca_topic_score_gemma":0.009935851,"teacher_disagreement_score":0.008090175,"about_ca_system_score_codex":0.0007043244,"about_ca_system_score_gemma":0.00018665064,"threshold_uncertainty_score":0.016086161},"labels":[],"label_agreement":null},{"id":"W2093534270","doi":"10.1088/0004-637x/758/1/44","title":"THE GALFA-H i COMPACT CLOUD CATALOG","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; University of Calgary","funders":"","keywords":"Galaxy; Population; Line (geometry); Molecular cloud; Galactic tide; Range (aeronautics); Milky Way; Solar mass","score_opus":0.013593765508079045,"score_gpt":0.25199150077767574,"score_spread":0.23839773526959668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093534270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5660853,0.0019506606,0.0020850238,0.0001773781,0.000052518742,0.00021250079,0.40151602,0.0021190452,0.025801565],"genre_scores_gemma":[0.37124085,0.00047197883,0.0033126364,0.00011543858,0.00008822818,0.00017175367,0.61907506,0.00010446735,0.0054195784],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997825,0.000015167312,0.000020377,0.000052185766,0.000062782936,0.00006697967],"domain_scores_gemma":[0.99876994,0.00010209115,0.00031293952,0.00032257012,0.00022995453,0.00026250936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030242998,0.00034776464,0.00023193109,0.007674374,0.00050635904,0.00082103256,0.0008417403,0.00019376773,0.009333002],"category_scores_gemma":[0.0013011651,0.00011621307,0.00023622297,0.0066015376,0.00014368644,0.0005346941,0.0007550238,0.00012726104,0.0042908234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071505806,0.00011911442,0.658986,0.00039313213,0.00015993736,0.00050898665,0.00045242716,0.0017694472,0.0070729917,0.0027244715,0.17287636,0.15422216],"study_design_scores_gemma":[0.000091125505,0.00008225707,0.793133,0.00008089118,0.000051295607,0.00069115206,0.00021311986,0.0024805064,0.0020162098,0.00069027394,0.20044665,0.000023511351],"about_ca_topic_score_codex":0.015838321,"about_ca_topic_score_gemma":0.015532372,"teacher_disagreement_score":0.015838321,"about_ca_system_score_codex":0.0005924414,"about_ca_system_score_gemma":0.00051138486,"threshold_uncertainty_score":0.031492293},"labels":[],"label_agreement":null},{"id":"W2093555107","doi":"10.1088/0004-637x/801/2/104","title":"WEATHER ON OTHER WORLDS. III. A SURVEY FOR T DWARFS WITH HIGH-AMPLITUDE OPTICAL VARIABILITY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Brown dwarf; Context (archaeology); Variable star; Variation (astronomy); Amplitude; Infrared; Telescope; Photometry (optics)","score_opus":0.024843315865169215,"score_gpt":0.2503211314824758,"score_spread":0.2254778156173066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093555107","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22889724,0.00613344,0.0036367336,0.011772274,0.0027197385,0.00018608225,0.018161928,0.0017042379,0.72678834],"genre_scores_gemma":[0.54389095,0.0050774007,0.0042288816,0.004479968,0.0013036213,0.00007892386,0.013288759,0.0006883737,0.42696312],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99977833,0.000027925027,0.000016903725,0.00005155578,0.00006395309,0.00006132867],"domain_scores_gemma":[0.9991522,0.00005014985,0.0001559284,0.00019896905,0.0001565872,0.00028614924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033382062,0.00019557454,0.00024648043,0.0006918019,0.0012808193,0.0022585562,0.00025393622,0.00037535327,0.0709985],"category_scores_gemma":[0.0009232888,0.00010146667,0.00018193606,0.0012311572,0.00041824093,0.0017058655,0.0012721592,0.0008259081,0.024555173],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046446687,0.00019687989,0.13370574,0.00045344495,0.00015076651,0.002305983,0.0059630764,0.0005192912,0.0083052525,0.027819997,0.43656772,0.38354746],"study_design_scores_gemma":[0.000012942756,0.000037966798,0.061459146,0.00009233911,0.000010675916,0.0004327391,0.002298261,0.00014136314,0.00049035536,0.0017541662,0.93325186,0.000018238728],"about_ca_topic_score_codex":0.006588467,"about_ca_topic_score_gemma":0.01372248,"teacher_disagreement_score":0.0709985,"about_ca_system_score_codex":0.0004859746,"about_ca_system_score_gemma":0.00045290196,"threshold_uncertainty_score":0.2375136},"labels":[],"label_agreement":null},{"id":"W2093625784","doi":"10.1088/0004-637x/757/2/114","title":"BROAD ABSORPTION LINE DISAPPEARANCE ON MULTI-YEAR TIMESCALES IN A LARGE QUASAR SAMPLE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Sky; Line (geometry); Outflow; Spectral line; Absorption (acoustics); Absorption spectroscopy; Emission spectrum","score_opus":0.012810511535287304,"score_gpt":0.24555972890934538,"score_spread":0.23274921737405807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093625784","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993955,0.00013140324,0.00008441554,0.000021246195,0.0000023703956,0.0000018571446,0.00018782157,0.0000072351504,0.00016811043],"genre_scores_gemma":[0.9991709,0.000058803846,0.000069481015,0.000021278156,0.000010055135,0.0000039451807,0.00035932963,0.0000063789007,0.0002999175],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984837,0.000017729713,0.00001024152,0.000064402426,0.000018898792,0.000040227435],"domain_scores_gemma":[0.9988354,0.0002562068,0.00040330566,0.00010339123,0.00012834425,0.00027336716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006022,0.000117820964,0.00031365833,0.0010017033,0.00037754793,0.0006392925,0.0002964482,0.0003974345,0.0016238303],"category_scores_gemma":[0.0011425877,0.00016890591,0.00027622902,0.0004958778,0.0002412498,0.0004684879,0.00045522847,0.00036273545,0.0004053919],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025329998,0.000087197106,0.97490793,0.000014466298,0.000069929934,0.00025074175,0.00030925355,0.000103124774,0.016086793,0.000047321922,0.0002659731,0.00760389],"study_design_scores_gemma":[0.0000013326711,0.000018960696,0.99957186,5.7334535e-7,0.000009273316,0.00010585366,0.000050283386,0.00004122486,0.00009813157,0.000010508837,0.00009037114,0.0000016366799],"about_ca_topic_score_codex":0.0018403605,"about_ca_topic_score_gemma":0.0029763158,"teacher_disagreement_score":0.0018403605,"about_ca_system_score_codex":0.00016554336,"about_ca_system_score_gemma":0.000108199994,"threshold_uncertainty_score":0.0054323077},"labels":[],"label_agreement":null},{"id":"W2093788401","doi":"10.1088/0004-637x/776/1/47","title":"BLACK HOLE-NEUTRON STAR MERGERS WITH A HOT NUCLEAR EQUATION OF STATE: OUTFLOW AND NEUTRINO-COOLED DISK FOR A LOW-MASS, HIGH-SPIN CASE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Neutron star; Neutrino; Astrophysics; Accretion (finance); Black hole (networking); Equation of state; Nuclear physics","score_opus":0.008640827057501927,"score_gpt":0.21176333688706092,"score_spread":0.20312250982955898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093788401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961892,0.00013333024,0.0009811902,0.00016561092,0.000010690906,0.000016081001,0.00012664717,0.000036435064,0.0023407263],"genre_scores_gemma":[0.99877304,0.000053532083,0.0005684002,0.00002733515,0.000013123907,0.000008828015,0.000109089066,0.00001742144,0.000429254],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983096,0.000052858195,0.0000082608685,0.000022756692,0.000019616691,0.00006552224],"domain_scores_gemma":[0.99933475,0.00022875605,0.00018637186,0.00004412533,0.00005270484,0.00015334247],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042707616,0.00054526154,0.0006845861,0.0005416979,0.000984875,0.0012835824,0.0009196032,0.0011375861,0.0018120455],"category_scores_gemma":[0.0016196396,0.00037333355,0.0009460891,0.00036096046,0.0009473943,0.00076438417,0.00086320017,0.0005608909,0.00020997759],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010975079,0.00033903643,0.083980314,0.00012345373,0.00016658222,0.005561936,0.0003758975,0.8705662,0.01549759,0.019191138,0.00094496395,0.002155322],"study_design_scores_gemma":[0.00030791987,0.00016892582,0.014885817,0.000011221523,0.000063071944,0.00027156866,0.00018510951,0.97965586,0.0018143477,0.0022205953,0.00038211912,0.0000335462],"about_ca_topic_score_codex":0.017017536,"about_ca_topic_score_gemma":0.008883396,"teacher_disagreement_score":0.017017536,"about_ca_system_score_codex":0.00096747995,"about_ca_system_score_gemma":0.00052832806,"threshold_uncertainty_score":0.03383696},"labels":[],"label_agreement":null},{"id":"W2093794358","doi":"10.1088/0004-637x/709/1/546","title":"ERRATUM: “RADIATIVE EFFICIENCY AND CONTENT OF EXTRAGALACTIC RADIO SOURCES: TOWARD A UNIVERSAL SCALING RELATION BETWEEN JET POWER AND RADIO POWER” (2008, ApJ, 686, 859)","year":2010,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Jet (fluid); Magnetic field; Radiative transfer; Astrophysical jet; Radio frequency; Radio galaxy; Synchrotron; Astrophysics; Equipartition theorem; Computational physics; Optics; Galaxy; Active galactic nucleus; Mechanics","score_opus":0.012965522478796471,"score_gpt":0.21723362426299347,"score_spread":0.204268101784197,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093794358","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.048965883,0.03268964,0.016125202,0.09457996,0.7446364,0.00021005844,0.019840159,0.0032864464,0.039666194],"genre_scores_gemma":[0.26543197,0.036678586,0.03767988,0.08729486,0.17318246,0.0005233464,0.041491788,0.0040488467,0.35366827],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99943537,0.000074965465,0.00011435219,0.00016050189,0.00018258794,0.000032166477],"domain_scores_gemma":[0.99392503,0.0014728907,0.0006900364,0.00054120936,0.003161847,0.00020889593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012127553,0.0017575076,0.0006665435,0.0026290768,0.0012398344,0.0018579458,0.0016256999,0.001670507,0.018873345],"category_scores_gemma":[0.012834758,0.00055307033,0.000720622,0.0022700725,0.0009947584,0.0017516639,0.0008453014,0.0022466122,0.016475074],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017494372,0.000037019006,0.014556686,0.00046185916,0.00010607636,0.000547286,0.00014475858,0.00042891456,0.0018425328,0.0022161016,0.9315246,0.047959153],"study_design_scores_gemma":[0.0001335629,0.00028703015,0.11091126,0.00073781866,0.00027233633,0.0024745988,0.00060283305,0.0029361951,0.0056180814,0.004677497,0.8711071,0.00024168863],"about_ca_topic_score_codex":0.0084358575,"about_ca_topic_score_gemma":0.0069952845,"teacher_disagreement_score":0.018873345,"about_ca_system_score_codex":0.0006936722,"about_ca_system_score_gemma":0.0006568243,"threshold_uncertainty_score":0.06313759},"labels":[],"label_agreement":null},{"id":"W2093966116","doi":"10.1086/374042","title":"Blue Straggler Stars: A Direct Comparison of Star Counts and Population Ratios in Six Galactic Globular Clusters","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Blue straggler; Astrophysics; Physics; Metallicity; Star cluster; Cluster (spacecraft); Horizontal branch; Population; Stellar density; Luminosity; Stars; Stellar population; Astronomy; Galaxy; Star formation; Demography","score_opus":0.013702490513527843,"score_gpt":0.24987275249595334,"score_spread":0.2361702619824255,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093966116","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997497,0.000021545662,0.000029505312,0.0000018025136,2.3398925e-7,9.5719e-7,0.00008494228,0.0000035655105,0.00010768311],"genre_scores_gemma":[0.9992798,0.000023968922,0.00013781525,0.0000030881738,0.0000014190576,0.0000021563164,0.0004386339,0.0000028133538,0.00011032435],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998455,0.000015734957,0.000011580696,0.000060958773,0.000040565803,0.000025708632],"domain_scores_gemma":[0.999676,0.00005235417,0.00008355185,0.000029224866,0.000047246478,0.00011168708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015925289,0.00014252207,0.00019254889,0.0017457147,0.0002456546,0.00031791738,0.00019623335,0.00023237975,0.0009969743],"category_scores_gemma":[0.0004758371,0.00010075607,0.0001199301,0.0008966825,0.00022180326,0.00020403926,0.0004416866,0.00009361753,0.00029472212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019698865,0.000020153502,0.97998375,0.0000144890955,0.000034645145,0.000054910794,0.00035342432,0.00017300039,0.014172827,0.00006935088,0.00009284086,0.00483363],"study_design_scores_gemma":[0.000002472588,0.000030136625,0.9989599,9.0365177e-7,0.000006214746,0.000081807106,0.00010599224,0.00011635531,0.0005677656,0.000016073984,0.00011078713,0.0000016438503],"about_ca_topic_score_codex":0.0036750361,"about_ca_topic_score_gemma":0.007856748,"teacher_disagreement_score":0.0036750361,"about_ca_system_score_codex":0.00021932136,"about_ca_system_score_gemma":0.000105850646,"threshold_uncertainty_score":0.007307291},"labels":[],"label_agreement":null},{"id":"W2093971048","doi":"10.1086/344475","title":"A Hyper Extremely Red Object in the Field near 53W002","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy; HERO; Stars; Redshift; Literature","score_opus":0.01259477640892822,"score_gpt":0.21223759504792758,"score_spread":0.19964281863899935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093971048","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9856861,0.00020958313,0.0010979067,0.00010648754,0.00002922094,0.000022233045,0.00059691584,0.00018051644,0.012071011],"genre_scores_gemma":[0.99362046,0.00012090737,0.0016596535,0.000117577125,0.000037085134,0.000015496124,0.001579351,0.000014902207,0.0028346058],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999304,0.000002983097,0.0000022795023,0.000021623397,0.000019885465,0.000022827753],"domain_scores_gemma":[0.9998252,0.000012485833,0.00004755978,0.00002205408,0.000013364784,0.00007941253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010941579,0.00023994478,0.00019905629,0.00073959125,0.00054624316,0.00044493694,0.0003247326,0.00048226738,0.0027835974],"category_scores_gemma":[0.00018283584,0.0001527162,0.00020073641,0.0006200582,0.00024988496,0.00027252774,0.0006968719,0.00036177228,0.0010120242],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051704457,0.0002369695,0.5325412,0.00021525637,0.0000843295,0.014155742,0.0012536147,0.00036605936,0.36120123,0.0028164252,0.009131012,0.077481166],"study_design_scores_gemma":[0.000020882657,0.00017030744,0.9718803,0.000025206933,0.000028260567,0.007020662,0.00028864347,0.00047127545,0.007446258,0.00028516562,0.012346964,0.000016039396],"about_ca_topic_score_codex":0.0017938099,"about_ca_topic_score_gemma":0.0024901894,"teacher_disagreement_score":0.0027835974,"about_ca_system_score_codex":0.00017816237,"about_ca_system_score_gemma":0.0001404098,"threshold_uncertainty_score":0.009312034},"labels":[],"label_agreement":null},{"id":"W2093975606","doi":"10.1086/375512","title":"Simulations of Galaxy Formation in a Λ Cold Dark Matter Universe. I. Dynamical and Photometric Properties of a Simulated Disk Galaxy","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":432,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy rotation curve; Astronomy; Lenticular galaxy; Galaxy; Galaxy formation and evolution; Interacting galaxy; Surface brightness; Cold dark matter; Dark matter halo; Halo","score_opus":0.008179915483086032,"score_gpt":0.2023280221632004,"score_spread":0.19414810668011437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093975606","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99262977,0.00009671077,0.0032553403,0.00012915228,0.000013523451,0.000043458258,0.0007554484,0.00012719932,0.0029494008],"genre_scores_gemma":[0.9935823,0.00009154424,0.00410391,0.00006648321,0.000010157992,0.000090080044,0.0009471315,0.000030188838,0.0010780203],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983203,0.00005882525,0.000009497609,0.000027036669,0.000021776328,0.000050774073],"domain_scores_gemma":[0.99875677,0.0005904975,0.00014114872,0.000098476165,0.00015067274,0.000262351],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043893672,0.0004454453,0.0005379874,0.00059721264,0.0005172429,0.00073316053,0.0012461661,0.0011191276,0.002206975],"category_scores_gemma":[0.0020154342,0.00033127706,0.0005978218,0.000623914,0.0006802548,0.00054041966,0.0008418285,0.0006741015,0.0002074811],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028133046,0.0001264041,0.021384023,0.000034833974,0.00006292309,0.00013970246,0.00013390617,0.9721586,0.0012526714,0.00272256,0.00035389498,0.0013491426],"study_design_scores_gemma":[0.00008594325,0.00007639337,0.0039165104,0.000007016574,0.00001562445,0.000023719633,0.00006277544,0.99403423,0.0003871865,0.00092579745,0.0004549685,0.000009777344],"about_ca_topic_score_codex":0.030435467,"about_ca_topic_score_gemma":0.01340846,"teacher_disagreement_score":0.030435467,"about_ca_system_score_codex":0.0013978919,"about_ca_system_score_gemma":0.0006078366,"threshold_uncertainty_score":0.060516655},"labels":[],"label_agreement":null},{"id":"W2093981711","doi":"10.1086/497117","title":"Mass‐to‐Light Ratios of Galaxy Groups from Weak Lensing","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Weak gravitational lensing; Galaxy; Mass ratio; RADIUS; Galaxy cluster; Redshift","score_opus":0.0067618162390316715,"score_gpt":0.20404948365913503,"score_spread":0.19728766742010337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093981711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937767,0.00004190447,0.00006704028,0.0000072759144,9.2730215e-7,0.0000024901929,0.00020035192,0.000005145667,0.00029727092],"genre_scores_gemma":[0.99905723,0.000024129222,0.000057403362,0.000004544716,0.0000046079017,0.0000033089918,0.000666165,0.0000047892945,0.00017777164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99943584,0.000049026952,0.00003587186,0.00012019024,0.00020315894,0.00015595971],"domain_scores_gemma":[0.99672675,0.00045172442,0.0011449408,0.0002883692,0.0005647796,0.00082341576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000495293,0.00043545078,0.00065075385,0.0038533167,0.00066431845,0.0010725044,0.00045075364,0.00028498736,0.0019272151],"category_scores_gemma":[0.0036831063,0.00021570823,0.00029125175,0.0016808106,0.0005430388,0.00040627262,0.0011637,0.000328433,0.00047001836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028572182,0.000022011645,0.9859934,0.00001807537,0.00007986843,0.000084193016,0.0004990967,0.00018400112,0.007542894,0.00010654339,0.00015492718,0.005029222],"study_design_scores_gemma":[0.000003950461,0.000037878865,0.99862087,0.0000013166402,0.0000162674,0.000079912665,0.00016862406,0.00025695923,0.0005550245,0.00005613102,0.00019885262,0.0000043805335],"about_ca_topic_score_codex":0.014014606,"about_ca_topic_score_gemma":0.010097743,"teacher_disagreement_score":0.014014606,"about_ca_system_score_codex":0.00044861698,"about_ca_system_score_gemma":0.0001812763,"threshold_uncertainty_score":0.027866066},"labels":[],"label_agreement":null},{"id":"W2093984292","doi":"10.1086/318165","title":"Detection of New Infrared Spectral Features in Hydrogenated Amorphous Carbon","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Amorphous carbon; Absorption (acoustics); Spectral line; Amorphous solid; Astrochemistry; Infrared; Carbon fibers; Interstellar medium; Infrared spectroscopy; Analytical Chemistry (journal); Crystallography; Materials science; Raman spectroscopy; Chemistry; Astronomy; Organic chemistry; Optics; Galaxy","score_opus":0.0054041822310506036,"score_gpt":0.21025451471856454,"score_spread":0.20485033248751394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2093984292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99693143,0.0003330017,0.0016736435,0.000027331185,0.000005209556,0.000006221106,0.00012637198,0.0000642053,0.0008324832],"genre_scores_gemma":[0.997891,0.00006664772,0.0014696063,0.000026604164,0.0000051058464,0.000004739872,0.00017305644,0.000008562933,0.00035461786],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999316,0.0000048731904,0.0000018784023,0.000019473753,0.000022589906,0.000019488263],"domain_scores_gemma":[0.99977547,0.00006216828,0.000059464972,0.000016688398,0.000043296237,0.00004296643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000087469045,0.00016816043,0.00010090501,0.00036586213,0.00022373251,0.00022457798,0.00038166792,0.00034000608,0.0010669316],"category_scores_gemma":[0.00018063496,0.00013354857,0.00014601216,0.00024446019,0.00025899743,0.00017730621,0.00015185859,0.00049006374,0.00015926035],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045757748,0.000022547416,0.003830066,0.000023303293,0.000010674296,0.00018139633,0.000048295627,0.00008483279,0.99377865,0.0000532615,0.000035955934,0.0018852694],"study_design_scores_gemma":[0.000018005201,0.00027946493,0.19949746,0.0000128700085,0.000032847736,0.0008892488,0.0001395662,0.0021403988,0.7949446,0.00016976759,0.0018569046,0.000018929435],"about_ca_topic_score_codex":0.0006664196,"about_ca_topic_score_gemma":0.0009452539,"teacher_disagreement_score":0.0010669316,"about_ca_system_score_codex":0.00018470372,"about_ca_system_score_gemma":0.000068781235,"threshold_uncertainty_score":0.0035691857},"labels":[],"label_agreement":null},{"id":"W2094067612","doi":"10.1088/0004-637x/777/1/22","title":"MEASURING THE COOLING OF THE NEUTRON STAR IN CASSIOPEIA A WITH ALL<i>CHANDRA X-RAY OBSERVATORY</i>DETECTORS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Acis; Physics; Observatory; Astrophysics; Cassiopeia A; Supernova; Neutron star; Neutrino; Nuclear physics; Supernova remnant","score_opus":0.02257767408570079,"score_gpt":0.2655655370128717,"score_spread":0.24298786292717092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094067612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98860043,0.00027796693,0.0023241318,0.00013886245,0.000023585135,0.00003316038,0.0030202838,0.00029316437,0.0052884277],"genre_scores_gemma":[0.98829716,0.0002038207,0.007326627,0.00014102276,0.000037719798,0.000050097824,0.0033476313,0.000104209204,0.0004917427],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992737,0.0000510526,0.000036644273,0.00034359578,0.0001931654,0.00010179004],"domain_scores_gemma":[0.9980744,0.00019868849,0.00052153156,0.0004688212,0.00043296482,0.000303607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010548909,0.000669524,0.0004957063,0.0011837019,0.00092093466,0.00080487976,0.0007473781,0.00049010117,0.0008558929],"category_scores_gemma":[0.0017853014,0.00057420245,0.0007091752,0.0012589318,0.00051684317,0.0006184699,0.0010179877,0.00095510605,0.00039479215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058721314,0.000113753995,0.8683272,0.00014923702,0.00062678824,0.00033609167,0.00047968392,0.002285006,0.11406881,0.0006046351,0.0027554615,0.009666042],"study_design_scores_gemma":[0.0000299817,0.000077059354,0.97298807,0.000016725806,0.0001651195,0.00025740277,0.00006751385,0.0039921063,0.01937641,0.00014460058,0.0028561878,0.00002876103],"about_ca_topic_score_codex":0.023613928,"about_ca_topic_score_gemma":0.050013855,"teacher_disagreement_score":0.023613928,"about_ca_system_score_codex":0.0010002694,"about_ca_system_score_gemma":0.0005869175,"threshold_uncertainty_score":0.046952963},"labels":[],"label_agreement":null},{"id":"W2094195431","doi":"10.1088/0004-637x/704/2/1098","title":"NEAR-INFRARED OBSERVATIONS OF GQ LUP b USING THE GEMINI INTEGRAL FIELD SPECTROGRAPH NIFS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto; Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Integral field spectrograph; Spectrograph; Luminosity; Spectral line; Spectroscopy; Effective temperature; Surface gravity; Stars","score_opus":0.027539482534559536,"score_gpt":0.296081552409004,"score_spread":0.2685420698744445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094195431","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.991169,0.00036603244,0.0014338248,0.00014677807,0.000018770434,0.000027302125,0.001089194,0.00027891886,0.0054702237],"genre_scores_gemma":[0.98664165,0.0001796154,0.007880165,0.00011863908,0.00007256246,0.000022211661,0.004034348,0.000034882785,0.0010159939],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998721,0.000011211727,0.0000044186772,0.00003754096,0.000052043324,0.000022660819],"domain_scores_gemma":[0.99958414,0.00002303496,0.00007266741,0.00006006659,0.00008847947,0.00017151602],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040092782,0.00019686791,0.00021460436,0.0011011222,0.0007628785,0.00028221885,0.00036314494,0.0002932727,0.001243895],"category_scores_gemma":[0.00033672125,0.0001670819,0.00017266457,0.0004495474,0.00025900017,0.000389955,0.00047503063,0.00032197573,0.00045076845],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011140236,0.0004578146,0.41298798,0.00018727126,0.0001706468,0.00087608077,0.0011070875,0.001131158,0.5014133,0.0010570271,0.006507686,0.07298992],"study_design_scores_gemma":[0.00007237997,0.00026779427,0.97486943,0.000013891851,0.00004564242,0.00071956293,0.00010848933,0.0022294484,0.010325158,0.00041594298,0.01091628,0.000015999096],"about_ca_topic_score_codex":0.0035309908,"about_ca_topic_score_gemma":0.00523711,"teacher_disagreement_score":0.0035309908,"about_ca_system_score_codex":0.0002793206,"about_ca_system_score_gemma":0.00010087335,"threshold_uncertainty_score":0.007020831},"labels":[],"label_agreement":null},{"id":"W2094212119","doi":"10.1086/587932","title":"On the Nature of Seyfert Galaxies with High [O<scp>iii</scp>] λ5007 Blueshifts","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":194,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Blueshift; Astrophysics; Physics; Galaxy; Doubly ionized oxygen; Ionization; Astronomy; Emission spectrum; Spectral line; Optics","score_opus":0.0054558100323787665,"score_gpt":0.19007396747968336,"score_spread":0.1846181574473046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094212119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965405,0.000055581044,0.00007698625,0.0000055712308,3.9972937e-7,0.0000011143779,0.000039577873,0.000005959885,0.00016072206],"genre_scores_gemma":[0.9995919,0.00002882923,0.00009757352,0.00000436759,0.0000040521622,0.0000016009832,0.00018993426,0.0000022805154,0.00007950992],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996934,0.000033110056,0.000018218721,0.000080590566,0.00006810037,0.000106605105],"domain_scores_gemma":[0.99751616,0.000560496,0.001049663,0.0002330193,0.00026401776,0.00037672004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052120537,0.00031243256,0.00041034576,0.0016408992,0.0004143872,0.00075674645,0.00030030642,0.00031675355,0.0011145412],"category_scores_gemma":[0.001392278,0.00013478016,0.0001402836,0.0011935891,0.000606682,0.0004686492,0.0005436031,0.00019182981,0.00034043146],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015889535,0.00003578101,0.9780386,0.0000112306725,0.00002296125,0.00026422605,0.00033758354,0.00017086956,0.01651261,0.000112600304,0.000039560742,0.004295169],"study_design_scores_gemma":[0.000002796775,0.00009067192,0.9979366,0.000002362335,0.0000069158496,0.00022921091,0.00019961022,0.0002176451,0.0010379271,0.0000641915,0.00020833481,0.0000038073229],"about_ca_topic_score_codex":0.0014331404,"about_ca_topic_score_gemma":0.002330569,"teacher_disagreement_score":0.0016408992,"about_ca_system_score_codex":0.00017859644,"about_ca_system_score_gemma":0.00008069332,"threshold_uncertainty_score":0.003728509},"labels":[],"label_agreement":null},{"id":"W2094216915","doi":"10.1088/0004-637x/790/2/136","title":"FAINT X-RAY BINARIES AND THEIR OPTICAL COUNTERPARTS IN M31","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Star cluster; Star (game theory); Population; Cluster (spacecraft); RADIUS; Stellar population; Star formation; Globular cluster","score_opus":0.007998915169245554,"score_gpt":0.20939961078010227,"score_spread":0.20140069561085672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094216915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943393,0.00004765002,0.00004604084,0.000011490961,5.15478e-7,0.0000028531476,0.00012136961,0.0000036532288,0.00033246822],"genre_scores_gemma":[0.9991685,0.000040327643,0.00012499721,0.000009893483,0.0000021073645,0.0000035926055,0.00040033297,0.0000026615357,0.0002476149],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974436,0.000027501486,0.000023625835,0.0000776081,0.000054356078,0.000072575574],"domain_scores_gemma":[0.99922705,0.00007928014,0.00036731747,0.00009647559,0.00005908897,0.00017076319],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003110648,0.00015315236,0.00025775193,0.0011874377,0.000593131,0.00072538655,0.00025841434,0.00028982133,0.0019714134],"category_scores_gemma":[0.0011802416,0.00016836227,0.0001908239,0.0013612385,0.0004021663,0.00056470244,0.0011192285,0.0001990675,0.0008785329],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008724471,0.000021369717,0.99312735,0.000006433607,0.0000089405485,0.0000956888,0.0001881277,0.00012472796,0.0030394155,0.000136356,0.000098104494,0.0030662948],"study_design_scores_gemma":[0.0000013898274,0.00002007077,0.99917644,0.0000023452076,0.0000028227053,0.00013413317,0.00011487415,0.00019226629,0.00013675979,0.000063307954,0.00015347807,0.0000020624034],"about_ca_topic_score_codex":0.0058502406,"about_ca_topic_score_gemma":0.0076779085,"teacher_disagreement_score":0.0058502406,"about_ca_system_score_codex":0.00036833182,"about_ca_system_score_gemma":0.00025083116,"threshold_uncertainty_score":0.011632383},"labels":[],"label_agreement":null},{"id":"W2094238336","doi":"10.1086/507174","title":"Extinction Columns and Intrinsic X‐Ray Spectra of the Anomalous X‐Ray Pulsars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Spectral line; Pulsar; Extinction (optical mineralogy); Halo; Range (aeronautics); Absorption (acoustics); Optical depth; Scattering; Interstellar medium","score_opus":0.006161594604958443,"score_gpt":0.19950345568964606,"score_spread":0.19334186108468762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094238336","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982698,0.0000642986,0.00037459092,0.000010259783,9.224325e-7,0.0000010536861,0.00012985652,0.000018348534,0.0011307896],"genre_scores_gemma":[0.99926907,0.000058611473,0.000238206,0.000010099873,0.0000024941928,0.0000024807991,0.00024321946,0.0000062646504,0.00016965697],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994254,0.000005948384,0.0000046153646,0.000019409554,0.000015169436,0.000012257481],"domain_scores_gemma":[0.9996966,0.00007690389,0.000092444636,0.00002844264,0.000065051114,0.00004052025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015607757,0.00019791698,0.00008880036,0.00066373625,0.00014289955,0.00044465114,0.00022291314,0.00013095286,0.0008703193],"category_scores_gemma":[0.00089426665,0.00016940058,0.00010561915,0.0003311236,0.00029283937,0.00042104637,0.00023348288,0.0001872951,0.00017964355],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004505275,0.00002290678,0.9495341,0.000023407234,0.00007344654,0.00011130838,0.00018749293,0.00448882,0.034799665,0.0011851162,0.00021155943,0.0093170805],"study_design_scores_gemma":[0.0000015869767,0.000014882619,0.992428,0.0000032626933,0.000008268429,0.000108745815,0.0000496716,0.0034692758,0.0034688818,0.0002389536,0.00020530251,0.0000031978666],"about_ca_topic_score_codex":0.0016672029,"about_ca_topic_score_gemma":0.0013788844,"teacher_disagreement_score":0.0016672029,"about_ca_system_score_codex":0.00018900333,"about_ca_system_score_gemma":0.000048349375,"threshold_uncertainty_score":0.003314972},"labels":[],"label_agreement":null},{"id":"W2094353177","doi":"10.1086/312560","title":"Caltech Faint Galaxy Redshift Survey. XI. The Merger Rate to Redshift 1 from Kinematic Pairs","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy; Redshift survey; Luminosity; Galaxy formation and evolution; Astronomy; Population","score_opus":0.010872049811443109,"score_gpt":0.2221406738914921,"score_spread":0.211268624080049,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094353177","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.05417068,0.00044542793,0.0012599207,0.0004976344,0.000063932835,0.0003040577,0.9077917,0.0007534851,0.034713093],"genre_scores_gemma":[0.08036201,0.00036142181,0.003661936,0.00033747882,0.000060041966,0.00032464231,0.8907731,0.000108141416,0.02401132],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99963164,0.000022676684,0.000019076426,0.00008963843,0.00015979048,0.00007716483],"domain_scores_gemma":[0.9985483,0.000058263795,0.00033635754,0.0001668688,0.00065891293,0.00023120493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057430455,0.00059433916,0.00041348714,0.0042741215,0.00082644343,0.0008311444,0.0006825257,0.0003605273,0.014303377],"category_scores_gemma":[0.0012548245,0.00026359243,0.0003057757,0.004795704,0.00013819122,0.00047967955,0.0007522015,0.0007891065,0.0104856575],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023049346,0.000104500956,0.35886115,0.00020108368,0.00011713904,0.00010690875,0.00026426933,0.00050471403,0.0010242771,0.0033222437,0.580442,0.054821227],"study_design_scores_gemma":[0.000068746755,0.00002911923,0.85481054,0.000023323106,0.0000312354,0.000085071966,0.00009571396,0.00084188045,0.0004446905,0.0004090082,0.14315051,0.000010179591],"about_ca_topic_score_codex":0.30221668,"about_ca_topic_score_gemma":0.40785316,"teacher_disagreement_score":0.30221668,"about_ca_system_score_codex":0.0021610158,"about_ca_system_score_gemma":0.0012537135,"threshold_uncertainty_score":0.6009152},"labels":[],"label_agreement":null},{"id":"W2094406252","doi":"10.1088/0004-637x/707/2/890","title":"<i>SPITZER</i>OBSERVATIONS OF PASSIVE AND STAR-FORMING EARLY-TYPE GALAXIES: AN INFRARED COLOR–COLOR SEQUENCE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Galaxy; Luminous infrared galaxy; Luminosity; Star formation; Infrared; Stellar mass; Peculiar galaxy; Elliptical galaxy","score_opus":0.017042942250035158,"score_gpt":0.23599968567877289,"score_spread":0.21895674342873772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094406252","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9862061,0.0004636583,0.0015818219,0.00011733038,0.000008274041,0.000025044365,0.005903195,0.00033830115,0.005356376],"genre_scores_gemma":[0.97978574,0.00041473698,0.0044826074,0.00014168523,0.00009369708,0.00003012527,0.012866725,0.000043951517,0.0021408119],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993837,0.0000059817694,0.000004560922,0.000013982359,0.000020914576,0.000016244156],"domain_scores_gemma":[0.9996687,0.000033083135,0.00013638436,0.000036623886,0.000055036566,0.00007023854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001672118,0.00023431984,0.00010190291,0.0026277134,0.0001608328,0.0003224783,0.00020068667,0.00014551943,0.0017203587],"category_scores_gemma":[0.00026535752,0.00007705847,0.00013670603,0.0011954921,0.0001475399,0.0002734087,0.00029793402,0.00013039836,0.000609075],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014877188,0.00012399998,0.87713253,0.00011056545,0.000060927192,0.00035554907,0.0002550244,0.0005807936,0.07209819,0.00050171814,0.005219817,0.043412045],"study_design_scores_gemma":[0.0000016616214,0.0000255754,0.9956832,0.0000033389756,0.000005839911,0.00020310984,0.00001951282,0.00014136037,0.0015496806,0.000056643104,0.0023069251,0.0000032669952],"about_ca_topic_score_codex":0.00252443,"about_ca_topic_score_gemma":0.006787746,"teacher_disagreement_score":0.0026277134,"about_ca_system_score_codex":0.00014269965,"about_ca_system_score_gemma":0.00008326919,"threshold_uncertainty_score":0.005755186},"labels":[],"label_agreement":null},{"id":"W2094464523","doi":"10.1086/323256","title":"The Giant Flare of 1998 August 27 from SGR 1900+14. II. Radiative Mechanism and Physical Constraints on the Source","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":366,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Magnetar; Physics; Astrophysics; Flare; Neutron star; Magnetic field; Radiative transfer; Solar flare","score_opus":0.011723878327480116,"score_gpt":0.27846491298979925,"score_spread":0.26674103466231913,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094464523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995252,0.0003612997,0.00044753565,0.0001010623,0.000011792196,0.00001232248,0.0005049825,0.000049112037,0.003259969],"genre_scores_gemma":[0.99706334,0.00024085029,0.00061445765,0.000058934485,0.000054332457,0.000011682139,0.0015706184,0.000015825104,0.00036984496],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999974,0.0000014908591,0.0000015430678,0.0000066716593,0.000005665858,0.000010612265],"domain_scores_gemma":[0.9998934,0.0000137041225,0.000056512825,0.000008357365,0.000008504158,0.000019494826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008726876,0.00030826958,0.0001751951,0.00038684483,0.0002834031,0.00028968957,0.0002436648,0.00026591116,0.0008072324],"category_scores_gemma":[0.00021367414,0.000088991525,0.00023737714,0.00022236907,0.00020868302,0.00017828337,0.0003415097,0.00024367202,0.00016120174],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012501983,0.00012683799,0.7911142,0.00028966257,0.00012474752,0.004128113,0.0006000978,0.009072063,0.13201922,0.0058790357,0.005418449,0.049977366],"study_design_scores_gemma":[0.000032148713,0.00010204007,0.98869145,0.000024618404,0.000022592001,0.0009365464,0.00009380992,0.0034615246,0.0020940246,0.00071903,0.0038100455,0.000012090435],"about_ca_topic_score_codex":0.0037557096,"about_ca_topic_score_gemma":0.0055702785,"teacher_disagreement_score":0.0037557096,"about_ca_system_score_codex":0.00055661733,"about_ca_system_score_gemma":0.000083596664,"threshold_uncertainty_score":0.007467687},"labels":[],"label_agreement":null},{"id":"W2094616227","doi":"10.1088/0004-637x/693/2/1128","title":"PULSED VERY HIGH ENERGY γ-RAY EMISSION CONSTRAINTS FOR PSR B1951+32 FROM STACEE OBSERVATIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; TRIUMF","funders":"","keywords":"Physics; Cherenkov radiation; Pulsar; Gamma ray; Astrophysics; Telescope; Gamma-ray astronomy; Range (aeronautics); Cherenkov Telescope Array; Photon; High energy; Energy (signal processing); Astronomy; Detector; Optics; Atomic physics","score_opus":0.013908513983526995,"score_gpt":0.2228258574112531,"score_spread":0.2089173434277261,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094616227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940253,0.0006404152,0.0011768517,0.00010759481,0.0000073382485,0.000022289154,0.0008188672,0.00006857579,0.0031328003],"genre_scores_gemma":[0.99513465,0.00026779328,0.0015712786,0.00007632668,0.000016112355,0.000026717758,0.002589237,0.000017985965,0.00029977184],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972063,0.00002858969,0.000025178368,0.00006790598,0.00007549827,0.00008211689],"domain_scores_gemma":[0.998828,0.00027173385,0.00029702924,0.00020618671,0.00009837251,0.00029859843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081024173,0.0007056355,0.0006016716,0.0025792206,0.00076697837,0.0012577866,0.0007048445,0.000583356,0.003622047],"category_scores_gemma":[0.0017819419,0.0006029983,0.00038749387,0.0011786041,0.00042446298,0.0004969875,0.0015081356,0.0005193747,0.0009640942],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014702379,0.0002899371,0.55037403,0.0004383112,0.00023246286,0.0028797241,0.0010395763,0.0066230814,0.38778868,0.007112845,0.0042839157,0.037467163],"study_design_scores_gemma":[0.00024937047,0.00021920902,0.9542648,0.0001671173,0.0001540924,0.0014449265,0.000370052,0.009281031,0.019355042,0.0037069537,0.010708524,0.00007888515],"about_ca_topic_score_codex":0.0048744646,"about_ca_topic_score_gemma":0.011854473,"teacher_disagreement_score":0.0048744646,"about_ca_system_score_codex":0.00059639843,"about_ca_system_score_gemma":0.0004641,"threshold_uncertainty_score":0.012116969},"labels":[],"label_agreement":null},{"id":"W2094666834","doi":"10.1088/0004-637x/769/1/12","title":"LINE EMISSION FROM RADIATION-PRESSURIZED H II REGIONS. II. DYNAMICS AND POPULATION SYNTHESIS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Radiation pressure; Population; Emission spectrum; Radiation; Line (geometry); Star formation; COSMIC cancer database; Active galactic nucleus; Spectral line; Astronomy; Geometry; Optics","score_opus":0.005523151435177334,"score_gpt":0.20050795175013328,"score_spread":0.19498480031495594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094666834","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86057127,0.00027406958,0.12345123,0.00018581495,0.000045953355,0.00023981636,0.0057421247,0.0008801589,0.008609466],"genre_scores_gemma":[0.9482295,0.00027974794,0.04587765,0.00006489597,0.000016584707,0.0002475382,0.0033310591,0.0001640066,0.0017889232],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998753,0.000037042548,0.000008110648,0.000043538825,0.000021114762,0.000014856687],"domain_scores_gemma":[0.99949396,0.0002126275,0.00009393539,0.000091084825,0.00007209368,0.000036321333],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032979317,0.00031721743,0.00030648173,0.00042812314,0.000285482,0.0006582036,0.0010385381,0.0004680248,0.00272473],"category_scores_gemma":[0.0017882856,0.0003526727,0.00066190085,0.000434505,0.00031771287,0.00068651483,0.00049678003,0.00040465585,0.0004988993],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010271538,0.00008759476,0.07185644,0.0001279016,0.00009091214,0.00015222159,0.000218101,0.8850113,0.011213408,0.013057401,0.0009754319,0.0171066],"study_design_scores_gemma":[0.00004673437,0.000045753673,0.012162457,0.000010891283,0.000029357989,0.00008277663,0.000058501762,0.9726961,0.005891463,0.0062306407,0.0027281065,0.000017203522],"about_ca_topic_score_codex":0.007049936,"about_ca_topic_score_gemma":0.0046329163,"teacher_disagreement_score":0.007049936,"about_ca_system_score_codex":0.0010957379,"about_ca_system_score_gemma":0.00042822008,"threshold_uncertainty_score":0.01401782},"labels":[],"label_agreement":null},{"id":"W2094819464","doi":"10.1086/510183","title":"Pulsations Detected from Accreting High‐Mass X‐Ray Binaries at Low Luminosities","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Neutron star; Luminosity; Pulsar; Accretion (finance); Low Mass; Observatory; Astronomy; X-ray binary; Angular momentum; Stars; Galaxy","score_opus":0.009339421658166897,"score_gpt":0.21868103116025972,"score_spread":0.20934160950209282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094819464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938893,0.00006597718,0.00019730405,0.000009733054,0.000002759519,0.0000022267445,0.00002838593,0.000010373893,0.00029440527],"genre_scores_gemma":[0.9993825,0.000030494035,0.00026389793,0.000013706619,0.0000061694614,0.000003094175,0.0001360118,0.0000026747227,0.00016148566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981624,0.000017754795,0.000017367041,0.000050657192,0.00004096168,0.000056936624],"domain_scores_gemma":[0.99942005,0.00011588189,0.000248497,0.0000569266,0.0000437205,0.00011494095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027774667,0.0002328415,0.00034753294,0.00079294405,0.0006219403,0.0010100622,0.00029208764,0.0005000386,0.0012614153],"category_scores_gemma":[0.0005813105,0.00019996999,0.00012100727,0.00054672314,0.00045825326,0.00031687255,0.000779859,0.00041615,0.00025669739],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072737073,0.00017920761,0.76158017,0.000055907873,0.000052141797,0.0011611214,0.0004682676,0.00016798446,0.21953088,0.00026593317,0.000121200464,0.015689818],"study_design_scores_gemma":[0.000029974768,0.00037614556,0.9707652,0.0000065260124,0.000047440615,0.0028408193,0.00014290716,0.00060822576,0.024357852,0.00020207296,0.0006070676,0.00001575248],"about_ca_topic_score_codex":0.0005583607,"about_ca_topic_score_gemma":0.0007124497,"teacher_disagreement_score":0.0012614153,"about_ca_system_score_codex":0.00018487814,"about_ca_system_score_gemma":0.000115827184,"threshold_uncertainty_score":0.00421983},"labels":[],"label_agreement":null},{"id":"W2094827573","doi":"10.1086/505387","title":"From Supermassive Black Holes to Dwarf Elliptical Nuclei: A Mass Continuum","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Supermassive black hole; Intermediate-mass black hole; Globular cluster; Galaxy; Galactic Center; Dwarf galaxy; Black hole (networking); Galactic nuclei; Stellar black hole","score_opus":0.005623119927118624,"score_gpt":0.20154007825623105,"score_spread":0.19591695832911243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094827573","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9542481,0.0021333296,0.0036975958,0.0008135739,0.00004538597,0.000020326375,0.00007818432,0.000119802215,0.038843803],"genre_scores_gemma":[0.99765295,0.00025959848,0.000606922,0.00019449166,0.00004851712,0.0000063403504,0.000032126143,0.0000053196245,0.0011938045],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989426,0.000016144842,0.000004910319,0.000028760609,0.000030309138,0.00002568195],"domain_scores_gemma":[0.99906904,0.00039027637,0.00017586889,0.00009859086,0.00005684418,0.00020939833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003372506,0.00022068925,0.00024350318,0.0007964745,0.00052486145,0.0012456926,0.00042999393,0.00052366883,0.0047114864],"category_scores_gemma":[0.001485276,0.00015273178,0.00012126335,0.00031383088,0.0015314047,0.0012923072,0.0014389305,0.00052195933,0.0005094415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015760701,0.0005675318,0.5489543,0.00027034158,0.000059221646,0.0050684777,0.0052569946,0.0011243906,0.055896454,0.21329616,0.005109297,0.16282076],"study_design_scores_gemma":[0.00030402886,0.0007260896,0.6887577,0.00017854654,0.00004977436,0.018154724,0.0025042398,0.0053996337,0.011105045,0.23944904,0.033319995,0.000051264382],"about_ca_topic_score_codex":0.00018691047,"about_ca_topic_score_gemma":0.000227849,"teacher_disagreement_score":0.0047114864,"about_ca_system_score_codex":0.0003205405,"about_ca_system_score_gemma":0.00009342677,"threshold_uncertainty_score":0.015761495},"labels":[],"label_agreement":null},{"id":"W2094883172","doi":"10.1086/345294","title":"Large‐Scale Turbulence in Molecular Clouds","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Molecular cloud; Turbulence; Physics; Astrophysics; Scale (ratio); Dissipation; Shock (circulatory); Computational physics; Mechanics; Statistical physics; Stars","score_opus":0.005881927285291848,"score_gpt":0.2278923720154665,"score_spread":0.22201044473017464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094883172","genre_codex":"editorial","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.20483544,0.019645639,0.003721251,0.16781673,0.32068488,0.0006205611,0.0034990355,0.0013847343,0.2777917],"genre_scores_gemma":[0.422282,0.011786714,0.0012684197,0.0052844896,0.08139964,0.0001383037,0.003227617,0.0004805518,0.47413233],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99888533,0.00014444222,0.00006910397,0.000120429955,0.00065891974,0.000121796686],"domain_scores_gemma":[0.9760395,0.0023619523,0.0008712769,0.0009956821,0.017476758,0.0022548204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015811439,0.00024090458,0.000862022,0.0015385777,0.0017102675,0.0027596753,0.0007618745,0.0018640228,0.08778506],"category_scores_gemma":[0.016843019,0.0002101925,0.000302855,0.0009804509,0.00064501853,0.0012661705,0.0008448891,0.0005997399,0.021238131],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004832784,0.00006770279,0.008303517,0.0010678442,0.000054891687,0.00087391987,0.00026098252,0.0005142402,0.0034447133,0.0036682934,0.8726737,0.1085869],"study_design_scores_gemma":[0.0002093325,0.00028206885,0.071365975,0.0005780853,0.00010261593,0.0008691308,0.0009647555,0.0047195093,0.0058931815,0.010578128,0.9043381,0.00009908718],"about_ca_topic_score_codex":0.0011125305,"about_ca_topic_score_gemma":0.0022719263,"teacher_disagreement_score":0.08778506,"about_ca_system_score_codex":0.0008808798,"about_ca_system_score_gemma":0.0012487873,"threshold_uncertainty_score":0.2936703},"labels":[],"label_agreement":null},{"id":"W2094963995","doi":"10.1088/0004-637x/802/1/30","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. VI. THE KINEMATICS OF ULTRA-COMPACT DWARFS AND GLOBULAR CLUSTERS IN M87","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Nautical Research Society; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Virgo Cluster; Star cluster; Astronomy; Dwarf galaxy; Galaxy; Galaxy cluster","score_opus":0.03003064314705959,"score_gpt":0.243093362938155,"score_spread":0.21306271979109542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094963995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7501118,0.0031878029,0.0006860791,0.0021685865,0.00010625103,0.00015163196,0.2198787,0.0003429949,0.023366133],"genre_scores_gemma":[0.8135909,0.0011425146,0.0022708552,0.00069720205,0.000058405243,0.00019194241,0.16536047,0.00006558166,0.016622104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998896,0.000015996444,0.00000787584,0.000021231292,0.000031094136,0.000034200064],"domain_scores_gemma":[0.9995938,0.000022490009,0.000069293004,0.000049627142,0.000091040856,0.00017369394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003063523,0.00011978861,0.00013852632,0.0020952057,0.00036066497,0.0004721439,0.0004517486,0.00026159306,0.0031332595],"category_scores_gemma":[0.0006874311,0.00010967443,0.00018262501,0.0016972666,0.00012313669,0.00025003558,0.0010656056,0.00021850503,0.0009904933],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016226883,0.00005634084,0.8891837,0.00010091733,0.00010805332,0.00013292128,0.0006497934,0.00039653137,0.0016883147,0.0013625522,0.065172546,0.040986083],"study_design_scores_gemma":[0.000005673466,0.0000041349454,0.98469526,0.000015741678,0.000010334105,0.000027745504,0.00017917766,0.000067627356,0.00007751216,0.00009091251,0.014823889,0.0000019164581],"about_ca_topic_score_codex":0.19556028,"about_ca_topic_score_gemma":0.31546372,"teacher_disagreement_score":0.19556028,"about_ca_system_score_codex":0.0009106069,"about_ca_system_score_gemma":0.0009276664,"threshold_uncertainty_score":0.38884395},"labels":[],"label_agreement":null},{"id":"W2094976523","doi":"10.1086/338952","title":"Models of Metal‐poor Stars with Gravitational Settling and Radiative Accelerations. I. Evolution and Abundance Anomalies","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Université de Montréal; Compute Canada","funders":"","keywords":"Physics; Astrophysics; Radiative transfer; Stars; Population; Settling; Astronomy","score_opus":0.01657141367350934,"score_gpt":0.21422160198243065,"score_spread":0.1976501883089213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2094976523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95034814,0.00068081863,0.029921569,0.0005360387,0.000052362415,0.00006287068,0.001594004,0.00035879062,0.016445395],"genre_scores_gemma":[0.97967726,0.0004192417,0.00592701,0.00015295504,0.000037312228,0.0001341899,0.0016608805,0.00017941614,0.011811788],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998709,0.000033023465,0.000006698166,0.000033329863,0.000016273634,0.000039699727],"domain_scores_gemma":[0.9997278,0.000055107936,0.00006270279,0.00002662981,0.000045922756,0.000081903265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003417139,0.00081089017,0.00058074587,0.0006514967,0.00079130864,0.0011520139,0.0017943343,0.0013698061,0.0017139162],"category_scores_gemma":[0.0007410411,0.00042798562,0.0013479873,0.00058339996,0.0004818391,0.0006309998,0.00086145947,0.00056076795,0.0009099654],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002571648,0.00006980268,0.041156903,0.00006495141,0.00013714605,0.00054261537,0.00040371288,0.9239156,0.0061994153,0.021468055,0.001699698,0.0040848344],"study_design_scores_gemma":[0.00008275196,0.00006956622,0.010367017,0.000019174711,0.000043376232,0.00023934324,0.000089484995,0.9750343,0.0006436173,0.009604131,0.0037737607,0.000033444354],"about_ca_topic_score_codex":0.011296884,"about_ca_topic_score_gemma":0.0045452807,"teacher_disagreement_score":0.011296884,"about_ca_system_score_codex":0.001372559,"about_ca_system_score_gemma":0.0003921311,"threshold_uncertainty_score":0.022462308},"labels":[],"label_agreement":null},{"id":"W2095058272","doi":"10.1086/518760","title":"Outflow and Infall in a Sample of Massive Star‐forming Regions","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Protostar; Outflow; James Clerk Maxwell Telescope; Accretion (finance); Star formation; High mass; Accretion disc; Stars","score_opus":0.012707761186748174,"score_gpt":0.2507528659336028,"score_spread":0.2380451047468546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095058272","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998301,0.00003775617,0.00002960338,0.000005094692,3.295822e-7,0.0000013703078,0.00003204007,0.0000015572438,0.00006212954],"genre_scores_gemma":[0.99962115,0.00004682748,0.00008700185,0.000009109124,0.0000036452118,0.0000018713405,0.00016978425,0.0000011050283,0.00005941255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982786,0.000025289488,0.000016274922,0.00004755737,0.0000283022,0.000054730313],"domain_scores_gemma":[0.9992187,0.00013401968,0.00032270554,0.000045673973,0.000044392178,0.00023442536],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028490095,0.00022559523,0.00026787864,0.0010940748,0.0005299321,0.000523358,0.0002540096,0.00026183235,0.00050921086],"category_scores_gemma":[0.00090844167,0.00019976245,0.00020755848,0.0006630477,0.00037456717,0.00022493178,0.00050960924,0.00016628738,0.00009652949],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046654623,0.000009505419,0.99677783,0.0000036617241,0.000009398576,0.00014602498,0.00019398908,0.000031320014,0.0015779227,0.000015455431,0.00001706976,0.0011711357],"study_design_scores_gemma":[0.0000013709465,0.000033273263,0.9991825,0.000001320752,0.0000057506204,0.00030543853,0.00012284188,0.00007883833,0.00019127913,0.000009421403,0.00006679179,0.0000011492228],"about_ca_topic_score_codex":0.0053315884,"about_ca_topic_score_gemma":0.009907821,"teacher_disagreement_score":0.0053315884,"about_ca_system_score_codex":0.00023560866,"about_ca_system_score_gemma":0.00014727257,"threshold_uncertainty_score":0.010601103},"labels":[],"label_agreement":null},{"id":"W2095072577","doi":"10.1086/586888","title":"Chemical Abundances of the Secondary Star in the Black Hole X‐Ray Binary XTE J1118+480","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Impact","funders":"","keywords":"Halo; Supernova; Black hole (networking); Galactic halo; Binary black hole; Spectral line; Stellar black hole; Star formation; Binary number","score_opus":0.013552829210946922,"score_gpt":0.22078059835990446,"score_spread":0.20722776914895755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095072577","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951947,0.0000229396,0.000036360627,0.000005094352,5.3051014e-7,0.0000012777537,0.00013057204,0.0000053283366,0.0002784363],"genre_scores_gemma":[0.9991424,0.000031335356,0.00009647349,0.0000027460444,0.0000012225249,0.0000025821364,0.0005158792,0.0000037788266,0.00020351248],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999573,0.000003185804,0.000002471858,0.000014156112,0.0000074990344,0.000015281099],"domain_scores_gemma":[0.9999052,0.000017875343,0.000027172759,0.000008441249,0.000008924039,0.000032372445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007907815,0.00031968934,0.00025232116,0.0005129898,0.00028239514,0.00050163094,0.00030497913,0.00033858928,0.0018626757],"category_scores_gemma":[0.00024636177,0.00018276891,0.00025876518,0.0002753497,0.00022736745,0.00019565344,0.00042001167,0.0001820938,0.0003303426],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005848648,0.0003154611,0.8367115,0.00014601457,0.00011805386,0.0013368397,0.00039489142,0.037368696,0.1121621,0.0015400635,0.000563201,0.008758372],"study_design_scores_gemma":[0.00009311682,0.00049746915,0.8698619,0.00001414075,0.00007933577,0.00064095,0.0003670393,0.10955075,0.016709048,0.0009973523,0.0011509875,0.000037752347],"about_ca_topic_score_codex":0.0038141678,"about_ca_topic_score_gemma":0.0028322695,"teacher_disagreement_score":0.0038141678,"about_ca_system_score_codex":0.00031745978,"about_ca_system_score_gemma":0.000099951285,"threshold_uncertainty_score":0.007583916},"labels":[],"label_agreement":null},{"id":"W2095143495","doi":"10.1088/0004-637x/764/2/124","title":"THE INFLUENCE OF ORBITAL ECCENTRICITY ON TIDAL RADII OF STAR CLUSTERS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Orbital eccentricity; RADIUS; Eccentricity (behavior); Star cluster; Globular cluster; Tidal heating; Orbital elements; Cluster (spacecraft); Orbit (dynamics); Tidal force","score_opus":0.0064118226555576596,"score_gpt":0.2060987418209142,"score_spread":0.19968691916535655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095143495","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962366,0.000051960134,0.0010074392,0.00010527362,0.00001361767,0.000011831746,0.00010303847,0.000049753115,0.0024204],"genre_scores_gemma":[0.99894565,0.000029563316,0.000651952,0.000017286082,0.0000022365746,0.000008234999,0.00009323218,0.000028346132,0.00022341828],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.999676,0.00010935922,0.00001810974,0.00005379845,0.000055976598,0.00008673547],"domain_scores_gemma":[0.9979279,0.0012228994,0.0001702313,0.00018175806,0.00023857813,0.0002586932],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009416267,0.00039986914,0.0005306688,0.00043754288,0.0010271819,0.0009925705,0.00092142576,0.0007246549,0.0010542998],"category_scores_gemma":[0.0072486745,0.00034970103,0.0004112249,0.0005280511,0.0011275783,0.00074250327,0.0007412364,0.0006815539,0.00014732117],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002427112,0.00006735265,0.017941311,0.00002666654,0.000040430965,0.000150611,0.00011312444,0.9756031,0.0022417125,0.001767985,0.0002875568,0.0015174364],"study_design_scores_gemma":[0.00008783893,0.00017435935,0.006129974,0.000014544802,0.000026124852,0.000046302834,0.00016046216,0.989963,0.0020285645,0.00091934705,0.00042481278,0.000024585644],"about_ca_topic_score_codex":0.015734134,"about_ca_topic_score_gemma":0.010731214,"teacher_disagreement_score":0.015734134,"about_ca_system_score_codex":0.0009404795,"about_ca_system_score_gemma":0.00094729086,"threshold_uncertainty_score":0.031285107},"labels":[],"label_agreement":null},{"id":"W2095184311","doi":"10.1088/0004-637x/779/2/150","title":"VERITAS OBSERVATIONS OF THE MICROQUASAR CYGNUS X-3","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Gamma ray; Astrophysics; Telescope; Astronomy; Radiation; Nuclear physics","score_opus":0.012334364909900409,"score_gpt":0.20436191058887007,"score_spread":0.19202754567896965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095184311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99607253,0.0001663424,0.00037167262,0.00004116973,0.000008028132,0.000019786294,0.001060632,0.000053198586,0.002206662],"genre_scores_gemma":[0.994882,0.00013957775,0.0016127087,0.00005326407,0.000018099767,0.00002179284,0.0026175473,0.000030975167,0.0006238914],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975294,0.000020496824,0.000010494613,0.000068552756,0.000083954306,0.00006360606],"domain_scores_gemma":[0.99953234,0.00006833217,0.00018452731,0.00006596116,0.00007079111,0.00007804791],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041023604,0.000346232,0.00030308723,0.00088252855,0.00042291367,0.0005445064,0.00037727805,0.00036819282,0.0007841457],"category_scores_gemma":[0.0004472417,0.00020904228,0.00041900412,0.000757708,0.00030839394,0.0003038383,0.00062930136,0.00042436444,0.00020626745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017214073,0.00021007624,0.7922425,0.0002083204,0.0003643804,0.0022232607,0.0013101785,0.0070755775,0.16783164,0.0016430186,0.003305641,0.021863837],"study_design_scores_gemma":[0.00005007498,0.00018420545,0.98396516,0.000024481848,0.000060864542,0.00065319904,0.0001327972,0.0031409024,0.007563055,0.00029412628,0.0039021946,0.000029012728],"about_ca_topic_score_codex":0.0104840435,"about_ca_topic_score_gemma":0.0240024,"teacher_disagreement_score":0.0104840435,"about_ca_system_score_codex":0.00087416114,"about_ca_system_score_gemma":0.0003761327,"threshold_uncertainty_score":0.02084601},"labels":[],"label_agreement":null},{"id":"W2095275892","doi":"10.1088/0004-637x/721/1/174","title":"THE SIZE AND ORIGIN OF METAL-ENRICHED REGIONS IN THE INTERGALACTIC MEDIUM FROM SPECTRA OF BINARY QUASARS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Redshift; Quasar; Galaxy; Intergalactic travel; Halo; Astronomy; Line-of-sight; Correlation function (quantum field theory)","score_opus":0.008560002989085602,"score_gpt":0.2290627110483265,"score_spread":0.2205027080592409,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095275892","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988538,0.00017936858,0.0005080111,0.0000079392175,0.0000012687057,0.0000012772742,0.0001424689,0.000023466211,0.0002823436],"genre_scores_gemma":[0.99927646,0.00007479695,0.00038817752,0.0000029197852,0.0000035871767,0.0000012021794,0.000198979,0.0000041916715,0.000049710416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999515,0.0000030701337,0.000002704876,0.000017428229,0.000009075788,0.000016258642],"domain_scores_gemma":[0.99961025,0.00006385757,0.00019451581,0.00003170977,0.000032346667,0.000067493245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000094114395,0.00018682673,0.00010729093,0.0017922651,0.00016679331,0.0006879669,0.00028061654,0.00016854808,0.00082510896],"category_scores_gemma":[0.00037772502,0.00015927386,0.00014940981,0.0006853519,0.0002429781,0.00037974695,0.00052330364,0.00013723131,0.00016229306],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018641588,0.000029529921,0.880973,0.000046573892,0.00007158994,0.0004554795,0.00037137733,0.0016076154,0.103099816,0.0005019414,0.00013948609,0.01251722],"study_design_scores_gemma":[0.0000026438186,0.000014898161,0.99322754,0.000003786402,0.000019962503,0.0002195692,0.00009538656,0.002342877,0.0037214286,0.00013394709,0.00021281642,0.0000052496994],"about_ca_topic_score_codex":0.001389841,"about_ca_topic_score_gemma":0.0020630732,"teacher_disagreement_score":0.0017922651,"about_ca_system_score_codex":0.00019668667,"about_ca_system_score_gemma":0.000052453066,"threshold_uncertainty_score":0.0027635694},"labels":[],"label_agreement":null},{"id":"W2095405706","doi":"10.1086/321527","title":"Stellar Pollution in the Solar Neighborhood","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Metallicity; Stars; Main sequence; Open cluster; Stellar atmosphere; Stellar evolution; Stellar collision","score_opus":0.011459175148254834,"score_gpt":0.22400654202021889,"score_spread":0.21254736687196404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095405706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988426,0.00010999061,0.000030153298,0.000034036606,0.0000014745822,0.0000010394958,0.00007076837,0.0000022783606,0.0009077233],"genre_scores_gemma":[0.999488,0.000091863025,0.000034113895,0.000011825051,0.000003084343,8.0579764e-7,0.00011351611,0.0000013834164,0.0002553601],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998461,0.00003591781,0.000008510637,0.000048473026,0.000029127741,0.000031887463],"domain_scores_gemma":[0.999549,0.000057265843,0.0001682803,0.000032794338,0.00006678488,0.00012601184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014647876,0.00006919689,0.00037216535,0.00042200493,0.00068409345,0.00076492043,0.0001908925,0.00034489314,0.0017622665],"category_scores_gemma":[0.0010006413,0.00011450314,0.00010717937,0.0007046547,0.0002992278,0.00029696076,0.0006080301,0.00018304166,0.00032217902],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007232023,0.000028010845,0.9939322,0.000009425137,0.000028667147,0.00016319902,0.00041535462,0.000333188,0.00043739326,0.00029236975,0.00017022548,0.0041175126],"study_design_scores_gemma":[0.0000058622904,0.000065356835,0.9963468,0.0000079845695,0.000017008879,0.0003858783,0.00075962435,0.000647353,0.00013349192,0.0003457736,0.001282324,0.0000026100881],"about_ca_topic_score_codex":0.0114071965,"about_ca_topic_score_gemma":0.020881528,"teacher_disagreement_score":0.0114071965,"about_ca_system_score_codex":0.00042292173,"about_ca_system_score_gemma":0.00015078005,"threshold_uncertainty_score":0.022681594},"labels":[],"label_agreement":null},{"id":"W2095424597","doi":"10.1088/0004-637x/801/1/64","title":"THE PUZZLING EARLY DETECTION OF LOW VELOCITY<sup>56</sup>Ni DECAY LINES IN SN 2014J: HINTS OF A COMPACT REMNANT","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Superconducting Materials and Applications","field":"Engineering","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Nuclear physics","score_opus":0.020729460379651076,"score_gpt":0.2377107344895379,"score_spread":0.21698127410988682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095424597","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99109006,0.00052169844,0.0034979545,0.00013746646,0.0000323273,0.0000068147046,0.00023523088,0.00014889348,0.0043295077],"genre_scores_gemma":[0.99689204,0.00010395675,0.0019677696,0.000047087993,0.000012907414,0.000003918112,0.00025623097,0.000021214813,0.0006949919],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999554,0.00000244988,0.0000033567612,0.000015579,0.000011959277,0.000011283179],"domain_scores_gemma":[0.9996301,0.000060173705,0.00014058723,0.000054750442,0.00005558146,0.000058878075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019383963,0.00025646083,0.00019758796,0.00065159914,0.0003972892,0.00051053107,0.00033823325,0.0004879894,0.0019240022],"category_scores_gemma":[0.0005335532,0.00014946511,0.00018212003,0.00041298548,0.00049731846,0.00034810413,0.00035665854,0.00050147274,0.00048902386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007464227,0.00008033951,0.5196453,0.00017182677,0.000069059315,0.0035504294,0.0003359764,0.00040461612,0.44977176,0.0036912833,0.0007084905,0.020824593],"study_design_scores_gemma":[0.000021698945,0.00035736727,0.8429282,0.000038948816,0.00012311288,0.00994862,0.0004073019,0.0035609917,0.12753236,0.004376476,0.010665587,0.000039412404],"about_ca_topic_score_codex":0.00084310013,"about_ca_topic_score_gemma":0.0024303498,"teacher_disagreement_score":0.0019240022,"about_ca_system_score_codex":0.00022998908,"about_ca_system_score_gemma":0.000098568154,"threshold_uncertainty_score":0.006436467},"labels":[],"label_agreement":null},{"id":"W2095481755","doi":"10.1086/511514","title":"The Spatial Distribution of the Galactic First Stars. II. Smoothed Particle Hydrodynamics Approach","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Stars; Initial mass function; Astrophysics; Galaxy; Metallicity; Milky Way; Smoothed-particle hydrodynamics; Bulge; Galactic halo; Star formation; Supernova; Astronomy; Halo; Population","score_opus":0.005414967407369408,"score_gpt":0.1958943593293116,"score_spread":0.1904793919219422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095481755","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3842071,0.0064701186,0.57476616,0.002981348,0.00048996374,0.00009730877,0.002493662,0.0015967163,0.02689762],"genre_scores_gemma":[0.94977796,0.0021463903,0.036297575,0.00012676505,0.00023891054,0.000048084035,0.0012040399,0.00016592102,0.009994363],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999584,0.000009363743,0.0000019812599,0.000010201099,0.000011811959,0.000008255872],"domain_scores_gemma":[0.99974924,0.000089583686,0.00004524346,0.000040052422,0.000040865372,0.0000349488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032032607,0.00023528855,0.0004046564,0.0009604933,0.00022027134,0.00048357263,0.00084768,0.00045900609,0.0019378177],"category_scores_gemma":[0.0013351542,0.00024747697,0.0007039406,0.0007523248,0.00041239162,0.0005900419,0.00040065957,0.00038307684,0.0005899357],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001256838,0.000039672857,0.01712494,0.00023296071,0.00013246968,0.00026741854,0.00011296659,0.6826361,0.006816934,0.22746588,0.008137222,0.05690778],"study_design_scores_gemma":[0.000021418458,0.00001627989,0.010793754,0.000018487177,0.000021895457,0.00010085328,0.00002259088,0.9427387,0.00081686093,0.0414957,0.003930324,0.000023093571],"about_ca_topic_score_codex":0.01593801,"about_ca_topic_score_gemma":0.006028983,"teacher_disagreement_score":0.01593801,"about_ca_system_score_codex":0.00067876274,"about_ca_system_score_gemma":0.0006902122,"threshold_uncertainty_score":0.03169048},"labels":[],"label_agreement":null},{"id":"W2095563730","doi":"10.1086/525244","title":"From Mean Motion Resonances to Scattered Planets: Producing the Solar System, Eccentric Exoplanets, and Late Heavy Bombardments","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Planetary system; Dynamical friction; Celestial mechanics; Stars; Solar System; Mean motion; Planet","score_opus":0.01309593221242727,"score_gpt":0.20706926013692833,"score_spread":0.19397332792450106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095563730","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951013,0.00032908673,0.0009165015,0.00007894196,0.000002945068,0.0000026677947,0.000010979542,0.000010864839,0.0035466384],"genre_scores_gemma":[0.9992093,0.000101777856,0.00028203303,0.000009261407,0.000002742449,9.0361533e-7,0.0000098803375,0.0000029773432,0.00038102706],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999261,0.00001922494,0.0000035523922,0.000020016187,0.000015970125,0.000015122315],"domain_scores_gemma":[0.99950135,0.00017780995,0.00014531745,0.00008057469,0.000021744765,0.00007320663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018380472,0.00022379031,0.00019918672,0.00036292916,0.00058851397,0.0006316478,0.00034627705,0.00045875588,0.0014734897],"category_scores_gemma":[0.001092165,0.00011865393,0.00012375161,0.0002742169,0.00073833426,0.00038931853,0.0014237447,0.00036504882,0.00018959193],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014372927,0.00029142993,0.5730858,0.00025336922,0.00018063794,0.016085383,0.0065939524,0.015074643,0.27550477,0.039623562,0.0016492044,0.07021995],"study_design_scores_gemma":[0.00018633364,0.0016344575,0.6874611,0.00008033884,0.00022072681,0.045983218,0.005288534,0.0489771,0.15296671,0.037377633,0.019716868,0.00010704875],"about_ca_topic_score_codex":0.00068694155,"about_ca_topic_score_gemma":0.00093978224,"teacher_disagreement_score":0.0014734897,"about_ca_system_score_codex":0.00025030415,"about_ca_system_score_gemma":0.000052437263,"threshold_uncertainty_score":0.004929304},"labels":[],"label_agreement":null},{"id":"W2095578447","doi":"10.1088/0004-637x/790/2/149","title":"VERY-HIGH ENERGY OBSERVATIONS OF THE GALACTIC CENTER REGION BY VERITAS IN 2010-2012","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Science Foundation; Science Foundation Ireland; U.S. Department of Energy; Office of Science; Smithsonian Institution","keywords":"Physics; Galactic Center; Astrophysics; Cosmic ray; Fermi Gamma-ray Space Telescope; Astronomy; Dark matter; Gamma ray; Supermassive black hole; Zenith; Annihilation; Supernova; Galaxy; Nuclear physics","score_opus":0.009991502313569472,"score_gpt":0.19336855058152816,"score_spread":0.1833770482679587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095578447","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9797988,0.00048689087,0.0006798719,0.00015159232,0.000041604166,0.000024953702,0.0109599065,0.00026762113,0.007588856],"genre_scores_gemma":[0.98280543,0.00018088419,0.0022038317,0.000068387446,0.000031396947,0.000013499642,0.012440677,0.00004792012,0.0022079602],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999627,0.000023030434,0.0000137024435,0.00010759999,0.0001472983,0.000081309234],"domain_scores_gemma":[0.9993118,0.00004914421,0.0001831178,0.00009535298,0.00024954465,0.000111066445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038893812,0.0002737441,0.00030794676,0.0012430565,0.00048776736,0.0006903414,0.00042946183,0.0003261362,0.0016662761],"category_scores_gemma":[0.0006549344,0.00024306361,0.00022855416,0.0009849787,0.00025932954,0.0003511186,0.0008477402,0.00039203823,0.0005036146],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016408619,0.00013494368,0.79432046,0.00019090022,0.00033333938,0.0011726253,0.001684789,0.0016305802,0.13173117,0.0015908738,0.012861758,0.052707594],"study_design_scores_gemma":[0.00003685083,0.00007496535,0.98324674,0.00002803963,0.00005286673,0.00032587134,0.00019587301,0.00091260846,0.0050921435,0.00009728819,0.009920295,0.000016565724],"about_ca_topic_score_codex":0.069970615,"about_ca_topic_score_gemma":0.1833463,"teacher_disagreement_score":0.069970615,"about_ca_system_score_codex":0.001375631,"about_ca_system_score_gemma":0.00072837836,"threshold_uncertainty_score":0.13912666},"labels":[],"label_agreement":null},{"id":"W2095877063","doi":"10.1088/0004-637x/767/1/38","title":"THE ATACAMA COSMOLOGY TELESCOPE: RELATION BETWEEN GALAXY CLUSTER OPTICAL RICHNESS AND SUNYAEV-ZEL'DOVICH EFFECT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"SLAC National Accelerator Laboratory; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Office of International Science and Engineering; Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; University of Toronto; Government of Ontario; National Science Foundation; Compute Canada; Princeton University; Aspen Center for Physics; University of Pennsylvania; U.S. Department of Energy; Office of the Dean for Research, Princeton University","keywords":"Physics; Planck; South Pole Telescope; Astrophysics; Galaxy cluster; Flux (metallurgy); Cluster (spacecraft); Sky; Cosmology; Galaxy; Telescope; Astronomy","score_opus":0.005124780206087757,"score_gpt":0.21299222707019766,"score_spread":0.2078674468641099,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095877063","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961337,0.00013702363,0.00015256714,0.00005741278,0.000004587299,0.0000057032116,0.001266572,0.000019528967,0.002222863],"genre_scores_gemma":[0.99869835,0.00003277894,0.000115594754,0.00001071013,0.0000075813764,0.0000042809825,0.00091503083,0.0000053870244,0.00021027401],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972314,0.0000575733,0.00001770676,0.00008353102,0.000058625355,0.000059372782],"domain_scores_gemma":[0.9964504,0.0010663606,0.001199757,0.00027794554,0.00021486737,0.00079068623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050144905,0.00013404754,0.00018945186,0.0012552583,0.00041427166,0.00057996484,0.00037514057,0.00027385663,0.0030147904],"category_scores_gemma":[0.0018772582,0.00018487779,0.0001575513,0.0010829098,0.00042683847,0.0003133418,0.00062003126,0.00027530955,0.00028469705],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004868779,0.000011136686,0.99728775,0.000008484489,0.000036596077,0.000026324951,0.00008931123,0.0003042392,0.0005925007,0.00016048619,0.00044719438,0.0009873257],"study_design_scores_gemma":[0.0000015292746,0.0000022782388,0.99956864,0.0000012610532,0.0000031584998,0.000010985039,0.000030075982,0.00020235404,0.000037014484,0.000016821645,0.00012489912,9.99945e-7],"about_ca_topic_score_codex":0.03953665,"about_ca_topic_score_gemma":0.045034613,"teacher_disagreement_score":0.03953665,"about_ca_system_score_codex":0.0004696565,"about_ca_system_score_gemma":0.00024394422,"threshold_uncertainty_score":0.07861304},"labels":[],"label_agreement":null},{"id":"W2095917766","doi":"10.1086/519294","title":"Galaxy Luminosity Functions to<i>z</i>∼1 from DEEP2 and COMBO‐17: Implications for Red Galaxy Formation","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Aeronautics and Space Administration; California Institute of Technology; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; W. M. Keck Foundation; Jet Propulsion Laboratory; Space Telescope Science Institute; New Mexico State University; Eli Lilly and Company; National Science Foundation","keywords":"Physics; Astrophysics; Elliptical galaxy; Astronomy; Galaxy; Luminous infrared galaxy; Stellar mass; Lenticular galaxy; Galaxy group; Star formation","score_opus":0.011842772990419716,"score_gpt":0.23188303041978472,"score_spread":0.220040257429365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095917766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99075997,0.00061920774,0.00056407746,0.00022025997,0.000009599655,0.000005917798,0.0034853732,0.00012321341,0.0042124116],"genre_scores_gemma":[0.9956032,0.00012669766,0.00031047402,0.00006644896,0.00000877936,0.000006290892,0.003163899,0.000028823471,0.0006854341],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979407,0.0000143022435,0.000006782123,0.000051354513,0.000027148291,0.000106375956],"domain_scores_gemma":[0.9979001,0.0002944976,0.0007147524,0.00016727178,0.00034756833,0.00057575764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007348242,0.00037623796,0.000372352,0.002430811,0.00023348242,0.0009495015,0.0005705805,0.00034299397,0.002950731],"category_scores_gemma":[0.0014434479,0.00022012206,0.0004165096,0.0012807747,0.0005079817,0.00072313956,0.0009645168,0.00048635874,0.0006986204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017947819,0.000014778709,0.977123,0.000063805404,0.000056185978,0.00010602907,0.00030654235,0.00056268746,0.0023038294,0.0009806853,0.001171362,0.017131548],"study_design_scores_gemma":[0.0000065058352,0.000014500175,0.99726677,0.00001122809,0.000013103415,0.00004258198,0.00011200984,0.0007574763,0.00055640016,0.0002038195,0.001011711,0.0000039127126],"about_ca_topic_score_codex":0.01883761,"about_ca_topic_score_gemma":0.013457655,"teacher_disagreement_score":0.01883761,"about_ca_system_score_codex":0.00089468004,"about_ca_system_score_gemma":0.00030318147,"threshold_uncertainty_score":0.037455916},"labels":[],"label_agreement":null},{"id":"W2095932303","doi":"10.1088/0004-637x/701/2/1895","title":"THE ULTRAVIOLET SPECTRUM AND PHYSICAL PROPERTIES OF THE MASS DONOR STAR IN HD 226868 = Cygnus X-1","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Supergiant; Astrophysics; RADIUS; Spectral energy distribution; Astronomy; Luminosity; Extinction (optical mineralogy); Stars; Optics; Galaxy","score_opus":0.0099751494674621,"score_gpt":0.20714817809088473,"score_spread":0.19717302862342262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2095932303","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99934477,0.000047581605,0.0000388319,0.00000637224,6.0913015e-7,6.9820265e-7,0.00007783876,0.0000056612457,0.0004777237],"genre_scores_gemma":[0.9993161,0.000036854115,0.000102361315,0.000007659489,0.0000031078214,7.598045e-7,0.0002520153,0.0000014417662,0.0002797206],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999715,0.0000031435604,0.0000013559331,0.000008240092,0.0000071381864,0.000008601006],"domain_scores_gemma":[0.9999199,0.000012160517,0.000033312048,0.000004568935,0.0000062932536,0.000023828128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006613042,0.0001243134,0.00010889712,0.00041716007,0.00018257851,0.00026314147,0.00008530118,0.00014658217,0.0009049161],"category_scores_gemma":[0.0001400258,0.00004388498,0.00006972095,0.0003068109,0.0001244186,0.00010701699,0.00016801474,0.00011048553,0.00020964388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049598556,0.00017742788,0.8506608,0.000067168665,0.000041780655,0.0007822295,0.0004495709,0.00096737785,0.12874247,0.00040906153,0.00053516484,0.016670993],"study_design_scores_gemma":[0.0000023392151,0.000040217943,0.9966434,0.0000017952002,0.000006295393,0.00032673436,0.000061039544,0.00034804118,0.0022260079,0.000030354504,0.00031200593,0.0000017033902],"about_ca_topic_score_codex":0.0013498565,"about_ca_topic_score_gemma":0.0019981167,"teacher_disagreement_score":0.0013498565,"about_ca_system_score_codex":0.0001469061,"about_ca_system_score_gemma":0.000033743017,"threshold_uncertainty_score":0.0030272603},"labels":[],"label_agreement":null},{"id":"W2096094069","doi":"10.1086/340551","title":"Galaxy Clusters in Hubble Volume Simulations: Cosmological Constraints from Sky Survey Populations","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":363,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy cluster; Dark matter; Galaxy; Sky; Redshift; Cluster (spacecraft); Hubble's law; Intracluster medium; Scaling","score_opus":0.03220626094461443,"score_gpt":0.24483396163980767,"score_spread":0.21262770069519324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096094069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9747456,0.00013990815,0.013382009,0.0005323853,0.000037324688,0.000079505124,0.0018001408,0.00039195234,0.008891182],"genre_scores_gemma":[0.9840344,0.00013212312,0.01227181,0.00021915653,0.000028937202,0.00017325503,0.0016811617,0.00018673154,0.0012724716],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996171,0.00017648553,0.000016719603,0.000057356,0.000063126456,0.00006918302],"domain_scores_gemma":[0.9960509,0.002530506,0.00034762005,0.0003126267,0.00029243078,0.00046587022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014858525,0.0005999863,0.0007865027,0.00078064826,0.0009863188,0.0012602984,0.00208446,0.0012453811,0.0023977696],"category_scores_gemma":[0.007293999,0.00064480404,0.00072885567,0.0009393534,0.0010791405,0.0009122238,0.0010545257,0.0013568565,0.0003878492],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009683691,0.0000580065,0.0101430025,0.000015376027,0.000039552095,0.000055450782,0.000067881694,0.98308337,0.00021343317,0.004922305,0.00047817046,0.00082659535],"study_design_scores_gemma":[0.00003971199,0.000012948575,0.0012423996,0.0000045200118,0.0000057748734,0.000006743744,0.000027972043,0.996729,0.00007283474,0.0016075958,0.00024337636,0.0000071182703],"about_ca_topic_score_codex":0.06401667,"about_ca_topic_score_gemma":0.03883955,"teacher_disagreement_score":0.06401667,"about_ca_system_score_codex":0.0019020061,"about_ca_system_score_gemma":0.001606895,"threshold_uncertainty_score":0.1272881},"labels":[],"label_agreement":null},{"id":"W2096147217","doi":"10.1086/587500","title":"Metallicity Calibrations and the Mass‐Metallicity Relation for Star‐forming Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1478,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Metallicity; Astrophysics; Galaxy; Astronomy; Star (game theory)","score_opus":0.018205249319491905,"score_gpt":0.23410538102687942,"score_spread":0.2159001317073875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096147217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99810946,0.00013277945,0.00077669363,0.000037738886,0.0000021140595,0.0000047986564,0.00031810877,0.00006637538,0.0005519663],"genre_scores_gemma":[0.9984573,0.000038397742,0.00069762097,0.0000114328295,0.000004456381,0.0000034600046,0.0006891667,0.000023687926,0.00007456691],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99923587,0.00023360542,0.000050867064,0.00020885706,0.00020110563,0.000069694055],"domain_scores_gemma":[0.99027973,0.0046148365,0.0030557131,0.0013328152,0.0004857194,0.00023108942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020334066,0.00042040768,0.00022210336,0.0014734946,0.00026399258,0.00059866847,0.0005222679,0.00041350865,0.0009100751],"category_scores_gemma":[0.008993041,0.00024398981,0.0004214943,0.0014244206,0.0004721977,0.00049631734,0.00053511735,0.000357876,0.00042741178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000098972516,0.00002649833,0.9845552,0.000016277236,0.00009309248,0.000039807623,0.00010824168,0.0045352657,0.0036779032,0.00023358005,0.00018944358,0.006425753],"study_design_scores_gemma":[0.0000133320555,0.000043701875,0.9864633,0.000009626936,0.000030824973,0.00004572389,0.00005210018,0.009383544,0.0033076822,0.00019487037,0.00044687575,0.00000843277],"about_ca_topic_score_codex":0.0042218277,"about_ca_topic_score_gemma":0.0045654397,"teacher_disagreement_score":0.0042218277,"about_ca_system_score_codex":0.0006369572,"about_ca_system_score_gemma":0.0001512662,"threshold_uncertainty_score":0.01075387},"labels":[],"label_agreement":null},{"id":"W2096215021","doi":"10.1088/0004-637x/695/2/1233","title":"ON THE CONTRIBUTION OF LARGE-SCALE STRUCTURE TO STRONG GRAVITATIONAL LENSING","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Science and Technology Facilities Council; Agence Nationale de la Recherche; Deutsche Forschungsgemeinschaft","keywords":"Physics; Galaxy; Astrophysics; Gravitational lens; Strong gravitational lensing; Weak gravitational lensing; Population; Lens (geology); Dark matter; Elliptical galaxy; Astronomy; Optics; Redshift","score_opus":0.005313525520631736,"score_gpt":0.22343971162260617,"score_spread":0.21812618610197443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096215021","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99381894,0.00053927425,0.0036696645,0.0003661187,0.0000085656075,0.0000069738044,0.00012241234,0.00005492357,0.0014131595],"genre_scores_gemma":[0.9990509,0.00011122058,0.00058316416,0.00002198727,0.000017311431,0.0000015094323,0.00008804005,0.00001374272,0.00011203156],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991611,0.000341213,0.00003144245,0.00018957217,0.00012048228,0.00015614912],"domain_scores_gemma":[0.9620142,0.024795117,0.007086979,0.0027821285,0.0010986476,0.0022230183],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028986118,0.0006175858,0.0004657049,0.0013240983,0.0005196099,0.0018104771,0.00077588623,0.00056969037,0.0017997306],"category_scores_gemma":[0.026449181,0.00043932456,0.0005294174,0.0012246473,0.0012155893,0.0014319583,0.0012857212,0.0007629585,0.00022579299],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012475144,0.0000384898,0.96507907,0.00006140197,0.00035309064,0.00031877428,0.00012723912,0.017321784,0.0025826937,0.0030203487,0.00029705607,0.010675295],"study_design_scores_gemma":[0.000027712076,0.00017169358,0.8302307,0.000028412356,0.00018809308,0.0003587429,0.00023328933,0.15709706,0.0022260454,0.008684895,0.00069823966,0.00005515327],"about_ca_topic_score_codex":0.0059495294,"about_ca_topic_score_gemma":0.0063658203,"teacher_disagreement_score":0.0059495294,"about_ca_system_score_codex":0.00054777367,"about_ca_system_score_gemma":0.00039339007,"threshold_uncertainty_score":0.01532954},"labels":[],"label_agreement":null},{"id":"W2096221457","doi":"10.1088/0004-637x/768/2/169","title":"<i>FERMI</i>LAT PULSED DETECTION OF PSR J0737–3039A IN THE DOUBLE PULSAR SYSTEM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Centre National de la Recherche Scientifique; Vetenskapsrådet; Japan Aerospace Exploration Agency; U.S. Department of Energy; Commonwealth Scientific and Industrial Research Organisation; Centre National d’Etudes Spatiales; Institut National de Physique Nucléaire et de Physique des Particules; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration","keywords":"Physics; Pulsar; Astrophysics; Millisecond pulsar; Fermi Gamma-ray Space Telescope; Astronomy; Light curve; Binary pulsar; Magnetosphere; Gamma ray; Neutron star; Telescope; Plasma; Nuclear physics","score_opus":0.007597962274763001,"score_gpt":0.20543294903811368,"score_spread":0.19783498676335068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096221457","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965653,0.0004096363,0.00023562243,0.00013384542,0.000030889165,0.000007922621,0.00059096044,0.00003800132,0.0019879153],"genre_scores_gemma":[0.9984219,0.00010555577,0.00047389627,0.00009067787,0.00002589579,0.000005897301,0.0006203283,0.000007107312,0.0002486694],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983525,0.000013109955,0.00001566368,0.000048374553,0.00003860104,0.000049024427],"domain_scores_gemma":[0.9996159,0.000037012775,0.000096285505,0.000057500187,0.000063759966,0.00012950553],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021399994,0.00029042628,0.00029619815,0.0017398951,0.00075353304,0.0006315073,0.00031973506,0.0005499007,0.0009070285],"category_scores_gemma":[0.0003282671,0.00012077557,0.00019743995,0.0007383153,0.00046261682,0.00017845209,0.00059373275,0.0003074592,0.0005832893],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069728843,0.00014053457,0.7181338,0.00012543204,0.00016030033,0.009803866,0.00073843286,0.0002694151,0.23505764,0.0008077121,0.004430576,0.029635027],"study_design_scores_gemma":[0.000024148007,0.0002122832,0.96340805,0.000035539815,0.00008347235,0.010861683,0.0003450876,0.0005373509,0.017724123,0.00037131895,0.006368178,0.000028769711],"about_ca_topic_score_codex":0.005618651,"about_ca_topic_score_gemma":0.007906222,"teacher_disagreement_score":0.005618651,"about_ca_system_score_codex":0.0004151834,"about_ca_system_score_gemma":0.00029275953,"threshold_uncertainty_score":0.011171937},"labels":[],"label_agreement":null},{"id":"W2096317990","doi":"10.1088/0004-637x/696/1/713","title":"THE HE-RICH CORE-COLLAPSE SUPERNOVA 2007Y: OBSERVATIONS FROM X-RAY TO RADIO WAVELENGTHS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Supernova; Bolometer; Spectral line; Light curve; Spectroscopy; Wavelength; Emission spectrum; Asymmetry","score_opus":0.020352715236997814,"score_gpt":0.24412115672600415,"score_spread":0.22376844148900635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096317990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9909017,0.0013100804,0.0007823866,0.000028810708,0.000012409661,0.00006158611,0.002497617,0.0000732718,0.0043322635],"genre_scores_gemma":[0.9762323,0.0020915982,0.0035256043,0.00012712022,0.0000612089,0.000045388962,0.014874026,0.00008449132,0.002958279],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998431,0.000009388476,0.000009826999,0.000035365574,0.00006427722,0.0000380537],"domain_scores_gemma":[0.9996655,0.0000142602685,0.00009271439,0.000029850398,0.00007409402,0.00012354193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053032144,0.00048247888,0.0005292991,0.0013822707,0.00062293094,0.0005987544,0.00038618103,0.0002612461,0.0006106508],"category_scores_gemma":[0.00018378475,0.00020673308,0.00030623257,0.0009822176,0.00016973123,0.00027417354,0.00066424377,0.00046008173,0.00060739764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032645362,0.0004082122,0.88636166,0.00016467599,0.000191826,0.0008453858,0.00043441055,0.00044755207,0.07522126,0.00044729354,0.003211383,0.031939894],"study_design_scores_gemma":[0.000005170702,0.00014429342,0.9893668,0.0000128277925,0.000017028782,0.0007220442,0.00008284888,0.0002456975,0.0029554332,0.000034466535,0.006407789,0.0000056323265],"about_ca_topic_score_codex":0.005803517,"about_ca_topic_score_gemma":0.011156238,"teacher_disagreement_score":0.005803517,"about_ca_system_score_codex":0.00033952022,"about_ca_system_score_gemma":0.00050427584,"threshold_uncertainty_score":0.011539519},"labels":[],"label_agreement":null},{"id":"W2096622517","doi":"10.1086/431240","title":"Discovery of Strong Lensing by an Elliptical Galaxy at <i>z</i> = 0.0345","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Velocity dispersion; Gravitational lens; Einstein ring; Einstein radius; Galaxy; Strong gravitational lensing; Elliptical galaxy; Redshift; Position angle","score_opus":0.007704554017007788,"score_gpt":0.2155237765441528,"score_spread":0.20781922252714502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096622517","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976186,0.00016225979,0.00052184996,0.000051494626,0.000004198444,0.0000033458264,0.00006496699,0.00004131653,0.0015320336],"genre_scores_gemma":[0.99926347,0.000044249737,0.00044448968,0.000027791257,0.000007006996,8.1298504e-7,0.00007461423,0.000004104104,0.00013336077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998221,0.000018017168,0.00001298726,0.000042807693,0.000052855456,0.00005131664],"domain_scores_gemma":[0.9994023,0.00007476358,0.00018324688,0.000065467175,0.00008685126,0.00018745224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047754374,0.00026005824,0.00024026826,0.00078840635,0.00040452543,0.0007682021,0.00028619028,0.00027031984,0.0008624278],"category_scores_gemma":[0.0006149011,0.00024886377,0.00029643293,0.0005216517,0.0003414229,0.00029951154,0.000639213,0.0002454989,0.00025425846],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017880852,0.0000751995,0.9013518,0.00004923879,0.00016013488,0.0018173533,0.0009655043,0.00030796722,0.07652994,0.0017645125,0.00073488517,0.016064677],"study_design_scores_gemma":[0.000013376467,0.00018157353,0.9805104,0.0000103306975,0.00007396594,0.0025568674,0.00018515512,0.0013864093,0.010890232,0.00031784532,0.0038576724,0.000016082466],"about_ca_topic_score_codex":0.0026370587,"about_ca_topic_score_gemma":0.003393545,"teacher_disagreement_score":0.0026370587,"about_ca_system_score_codex":0.00031835717,"about_ca_system_score_gemma":0.000107958935,"threshold_uncertainty_score":0.00524348},"labels":[],"label_agreement":null},{"id":"W2096780719","doi":"10.1088/0004-637x/792/2/135","title":"THE CORE COLLAPSE SUPERNOVA RATE FROM THE SDSS-II SUPERNOVA SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Lawrence Berkeley National Laboratory; Fermilab; U.S. Naval Observatory; Georg-August-Universität Göttingen; Chinese Academy of Sciences; University of Cambridge; York University; Drexel University; University of Pittsburgh; Johns Hopkins University; Universität Basel; University of Washington; Ohio State University; U.S. Department of Energy; Princeton University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Science and Technology Facilities Council; Case Western Reserve University","keywords":"Supernova; Type II supernova; Redshift; Sky; Luminosity; Core (optical fiber); Star formation","score_opus":0.020027135062115342,"score_gpt":0.23964263146067635,"score_spread":0.219615496398561,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096780719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.951031,0.0006100506,0.001955185,0.000099458855,0.000027303233,0.000075226424,0.036224127,0.00025497453,0.009722636],"genre_scores_gemma":[0.92842513,0.0005431061,0.0018131001,0.00005559349,0.000038221126,0.00004913586,0.06758911,0.00005856117,0.0014280905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966025,0.00006206118,0.000032530188,0.0000613009,0.00013917913,0.000044621946],"domain_scores_gemma":[0.9981502,0.00015419659,0.0007474191,0.00018139054,0.00042370855,0.0003431686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000968338,0.00033185552,0.00023780437,0.003085673,0.00016756564,0.00056708266,0.00028628443,0.00014923327,0.0009485612],"category_scores_gemma":[0.002239702,0.00012678985,0.0003172298,0.0019911854,0.00019252612,0.00029559588,0.00072330254,0.00026295712,0.0006004468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004188879,0.000025788433,0.9850071,0.00003613523,0.00014004164,0.00003278608,0.00010612524,0.0013949687,0.00096562493,0.0008248872,0.0044731107,0.0069515416],"study_design_scores_gemma":[0.000004261642,0.000014903476,0.993814,0.000009095457,0.000018572295,0.00008447574,0.00003312013,0.0012563912,0.00048363558,0.00022084519,0.0040541883,0.0000064226138],"about_ca_topic_score_codex":0.021733558,"about_ca_topic_score_gemma":0.021371426,"teacher_disagreement_score":0.021733558,"about_ca_system_score_codex":0.00053635205,"about_ca_system_score_gemma":0.00035707344,"threshold_uncertainty_score":0.043214083},"labels":[],"label_agreement":null},{"id":"W2096881337","doi":"10.1088/0004-637x/702/2/1199","title":"STATISTICAL TOOLS FOR CLASSIFYING GALAXY GROUP DYNAMICS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McMaster University","funders":"","keywords":"Gaussian; Galaxy; Cosmology; Statistic; Statistical hypothesis testing; Redshift; Test statistic; Robustness (evolution)","score_opus":0.013023897661656342,"score_gpt":0.2414125917759076,"score_spread":0.22838869411425125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2096881337","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08110982,0.0016323637,0.90496165,0.001256897,0.00018923517,0.00063227996,0.0035060933,0.0027757406,0.00393588],"genre_scores_gemma":[0.62413746,0.00077924185,0.36797562,0.00041302975,0.0005206338,0.0017747872,0.0034626713,0.00035214075,0.0005844556],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.98046654,0.011837515,0.0014889691,0.0016827189,0.004135469,0.00038885223],"domain_scores_gemma":[0.72366434,0.24311903,0.014482791,0.012915778,0.0044746697,0.0013433921],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.031462967,0.0016393211,0.001604756,0.017630568,0.001291492,0.003257123,0.0024273193,0.0016941541,0.0039706873],"category_scores_gemma":[0.17288683,0.00058843713,0.0016301529,0.010793035,0.0041429433,0.004485207,0.0025971492,0.003056179,0.0006723874],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004012285,0.00037971538,0.2090814,0.0012319721,0.0021470326,0.0006452195,0.0013942815,0.18528798,0.0030324582,0.26256138,0.016572136,0.3172652],"study_design_scores_gemma":[0.00013825482,0.00053364673,0.04177861,0.00026042538,0.00023201623,0.00067754363,0.0008955901,0.5675115,0.002062819,0.3756936,0.010026366,0.00018960919],"about_ca_topic_score_codex":0.0036872886,"about_ca_topic_score_gemma":0.0023816843,"teacher_disagreement_score":0.031462967,"about_ca_system_score_codex":0.0016250939,"about_ca_system_score_gemma":0.001988583,"threshold_uncertainty_score":0.16639405},"labels":[],"label_agreement":null},{"id":"W2097111510","doi":"10.1088/0004-637x/785/1/44","title":"A 10<sup>10</sup>SOLAR MASS FLOW OF MOLECULAR GAS IN THE A1835 BRIGHTEST CLUSTER GALAXY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":146,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Solar mass; Outflow; Star formation; Astronomy; Galaxy cluster; Radio galaxy; RADIUS","score_opus":0.004384803062270081,"score_gpt":0.19044785679478207,"score_spread":0.186063053732512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097111510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973484,0.00023576015,0.00012780279,0.00013151934,0.00001219102,0.0000034316865,0.00023829205,0.00007140483,0.0018310248],"genre_scores_gemma":[0.9990896,0.00003974156,0.00029115795,0.00006085096,0.000025066338,0.0000017724292,0.00022917285,0.0000035454823,0.00025916556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999485,0.0000037404466,0.0000028375982,0.000015961727,0.000012584713,0.000016307431],"domain_scores_gemma":[0.9998202,0.00002188965,0.00006626304,0.0000117757645,0.000017055972,0.00006292047],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007861604,0.00013839996,0.000078411336,0.00041281484,0.00026505537,0.00046152205,0.00023172065,0.00022949379,0.002398412],"category_scores_gemma":[0.00023992626,0.000078547615,0.0000858765,0.00017938526,0.00021119656,0.0002894204,0.00017212062,0.00014318981,0.0004974702],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004636603,0.00010987788,0.826702,0.00009068294,0.000050800736,0.0009845775,0.00047727025,0.00060604024,0.13549317,0.0016794506,0.0049526673,0.028389828],"study_design_scores_gemma":[0.000012912334,0.00013336969,0.99053556,0.000008473722,0.000020057423,0.0005480234,0.00012906652,0.0008916995,0.0040165875,0.00028073104,0.003418814,0.000004662394],"about_ca_topic_score_codex":0.0028979394,"about_ca_topic_score_gemma":0.004514614,"teacher_disagreement_score":0.0028979394,"about_ca_system_score_codex":0.00033591266,"about_ca_system_score_gemma":0.00009166648,"threshold_uncertainty_score":0.008023441},"labels":[],"label_agreement":null},{"id":"W2097214356","doi":"10.1088/0004-637x/763/2/83","title":"<i>HERSCHEL</i>/PACS SPECTROSCOPIC SURVEY OF PROTOSTARS IN ORION: THE ORIGIN OF FAR-INFRARED CO EMISSION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Emission spectrum; Excited state; Spectral line; Envelope (radar); Rotational temperature; Line (geometry); Orion Nebula; Astrochemistry","score_opus":0.01787568958658722,"score_gpt":0.2717466898623323,"score_spread":0.2538710002757451,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097214356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966959,0.0002290109,0.00010805367,0.000029195546,0.0000044087005,0.000005984053,0.0014965449,0.000038434104,0.0013925746],"genre_scores_gemma":[0.9935888,0.00023514553,0.0012239264,0.00003127735,0.000025903097,0.000009724218,0.0042784954,0.000022291439,0.00058444386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999889,0.000009773763,0.000007688361,0.000034344506,0.000034117136,0.000025021905],"domain_scores_gemma":[0.9996668,0.000025482224,0.00013544036,0.000042720054,0.000055900815,0.00007356255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020108334,0.00027134392,0.00015694404,0.0018916053,0.00030217663,0.0004379713,0.00018040037,0.00023952762,0.0010723803],"category_scores_gemma":[0.00027442956,0.00009643877,0.00017925976,0.0010601388,0.00019544347,0.0002563611,0.00045748337,0.00013403974,0.00031487172],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015058529,0.000048360784,0.94025624,0.00005182722,0.00008171034,0.00026006304,0.00021837562,0.0006020454,0.045904644,0.00015994263,0.0011252915,0.0111409705],"study_design_scores_gemma":[0.0000031369805,0.000014091039,0.99637693,0.0000032173157,0.000012970532,0.00013024545,0.000044316577,0.00027600824,0.0016000286,0.000024357883,0.0015112838,0.0000034533155],"about_ca_topic_score_codex":0.0054944158,"about_ca_topic_score_gemma":0.008768186,"teacher_disagreement_score":0.0054944158,"about_ca_system_score_codex":0.00033459137,"about_ca_system_score_gemma":0.00018696804,"threshold_uncertainty_score":0.010924876},"labels":[],"label_agreement":null},{"id":"W2097399791","doi":"10.1088/0004-637x/784/2/113","title":"DISCOVERY OF A POPULATION OF BULGELESS GALAXIES WITH EXTREMELY RED MID-IR COLORS: OBSCURED AGN ACTIVITY IN THE LOW-MASS REGIME?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Bulge; Supermassive black hole; Galaxy; Active galactic nucleus; Astronomy; Population; Sky; Luminous infrared galaxy; Stellar mass; Stellar population; Star formation","score_opus":0.007821054316882611,"score_gpt":0.20572610446979603,"score_spread":0.19790505015291343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097399791","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990681,0.0002544178,0.00023982214,0.000023509418,0.0000014691847,0.0000021183007,0.000062999236,0.000018539204,0.0003290615],"genre_scores_gemma":[0.9993284,0.00011355341,0.00023535299,0.00003850942,0.000007831375,0.000002027386,0.0001479896,0.0000025971672,0.00012378964],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998739,0.0000116152805,0.000006432768,0.00004960276,0.000025352014,0.00003302993],"domain_scores_gemma":[0.99958736,0.0000637905,0.00017482108,0.000040893607,0.0000368495,0.000096384094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022825996,0.00016475818,0.00026223934,0.0010777048,0.0002486368,0.0006953726,0.00031501977,0.00021801224,0.00074109156],"category_scores_gemma":[0.0004688035,0.000101151534,0.00011227145,0.0005141375,0.0004966896,0.000348889,0.0004779167,0.00021530467,0.00028972852],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009023895,0.000020878138,0.97131145,0.000022719874,0.00002866996,0.00032520195,0.00035484036,0.000032877888,0.017338086,0.00011532637,0.00013585722,0.010223808],"study_design_scores_gemma":[0.0000020270734,0.000037788737,0.997532,0.0000040630707,0.000013126064,0.00083872565,0.00024440288,0.00008196236,0.00088964764,0.000055913253,0.00029741516,0.000002942786],"about_ca_topic_score_codex":0.0010735599,"about_ca_topic_score_gemma":0.0019373408,"teacher_disagreement_score":0.0010777048,"about_ca_system_score_codex":0.0001411243,"about_ca_system_score_gemma":0.0000675905,"threshold_uncertainty_score":0.0024791956},"labels":[],"label_agreement":null},{"id":"W2097418627","doi":"10.1088/0004-637x/786/1/66","title":"BARIUM ISOTOPIC COMPOSITION OF MAINSTREAM SILICON CARBIDES FROM MURCHISON: CONSTRAINTS FOR<i>s</i>-PROCESS NUCLEOSYNTHESIS IN ASYMPTOTIC GIANT BRANCH STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Argonne National Laboratory; Natural Sciences and Engineering Research Council of Canada; Ministero dell’Istruzione, dell’Università e della Ricerca; University of Notre Dame; National Aeronautics and Space Administration; U.S. Department of Energy; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Asymptotic giant branch; Nucleosynthesis; Physics; s-process; Astrophysics; Stars; Murchison meteorite; Stellar nucleosynthesis; Barium; Astronomy; Chondrite; Chemistry","score_opus":0.006158233815533573,"score_gpt":0.20946001591811975,"score_spread":0.20330178210258618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097418627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989458,0.00010393584,0.0000956289,0.00000504369,0.0000018239809,0.0000021780827,0.00010073019,0.000007878677,0.00073698873],"genre_scores_gemma":[0.99867487,0.00006621422,0.000381199,0.000011260748,0.000003316712,0.0000023289494,0.00037670648,0.000014569143,0.00046954278],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999409,0.0000023358773,0.000003612726,0.000019102446,0.000023373823,0.000010700959],"domain_scores_gemma":[0.9999138,0.000008200851,0.000017736083,0.000010084688,0.000029184632,0.000020903375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006520284,0.0003231369,0.00034497175,0.00082029664,0.00041812414,0.00047582437,0.00024078379,0.00023887535,0.00085686066],"category_scores_gemma":[0.00012877998,0.00015037056,0.000217583,0.0004669079,0.00027945032,0.00014379156,0.00035977043,0.00018300676,0.00031591303],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006360884,0.000031136722,0.18566237,0.000060508642,0.000059171478,0.0008361085,0.00031993503,0.0005732048,0.79723024,0.00012231359,0.0001134959,0.014355411],"study_design_scores_gemma":[0.000024351726,0.00020481163,0.904021,0.000008727481,0.00005542921,0.00080372504,0.00030792097,0.0016630414,0.089891836,0.00009235705,0.0029142755,0.000012571469],"about_ca_topic_score_codex":0.012073283,"about_ca_topic_score_gemma":0.01987456,"teacher_disagreement_score":0.012073283,"about_ca_system_score_codex":0.00041246178,"about_ca_system_score_gemma":0.00013378794,"threshold_uncertainty_score":0.02400601},"labels":[],"label_agreement":null},{"id":"W2097486734","doi":"10.1088/0004-637x/702/2/1157","title":"VARIABLE SODIUM ABSORPTION IN A LOW-EXTINCTION TYPE Ia SUPERNOVA,","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"Jet Propulsion Laboratory; University of Texas at Austin; Carnegie Institution of Washington; U.S. Department of Energy; W. M. Keck Foundation; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Supernova; Astrophysics; Physics; Absorption (acoustics); Absorption spectroscopy; Extinction (optical mineralogy); Astronomy; Optics","score_opus":0.008444123631658562,"score_gpt":0.2312765247473818,"score_spread":0.22283240111572325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097486734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988612,0.00016957882,0.000364093,0.000009154161,0.0000057197058,0.0000026910232,0.00009776868,0.000015447507,0.00047434424],"genre_scores_gemma":[0.99884593,0.0000685263,0.0004767824,0.00001984169,0.000005000982,0.000002522559,0.0002979194,0.0000052853798,0.00027818416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999285,0.000005385431,0.000006969033,0.000027196438,0.000015872272,0.000016212638],"domain_scores_gemma":[0.9997613,0.00002338764,0.00010675153,0.000026684445,0.000026864718,0.00005503867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020758797,0.00015735373,0.0001730428,0.00032877916,0.00023630765,0.00049560255,0.00018671596,0.00030044184,0.0006632418],"category_scores_gemma":[0.00036329697,0.00013184069,0.00021218599,0.0002248728,0.00023483537,0.00021012498,0.0003196802,0.00023653172,0.00017382187],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002949033,0.00006019579,0.8074332,0.000044240387,0.00007631751,0.0005562782,0.00007029847,0.00012651335,0.18560518,0.00018980115,0.0001171005,0.0054260525],"study_design_scores_gemma":[0.00000502545,0.00015987128,0.98218095,0.0000044916096,0.00002844834,0.0014335794,0.000060411912,0.00032182023,0.014886928,0.00011995534,0.0007942887,0.000004226247],"about_ca_topic_score_codex":0.0013223006,"about_ca_topic_score_gemma":0.003680535,"teacher_disagreement_score":0.0013223006,"about_ca_system_score_codex":0.00018230836,"about_ca_system_score_gemma":0.00012496661,"threshold_uncertainty_score":0.00262928},"labels":[],"label_agreement":null},{"id":"W2097523063","doi":"10.1086/381430","title":"Constraints on the Very High Energy Emission from BL Lacertae Objects","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Flux (metallurgy); Egret; Observatory; Telescope; Astronomy; Redshift; Gamma ray; BL Lac object; Crab Nebula; Extragalactic background light; Synchrotron; Blazar; Galaxy; Nuclear physics","score_opus":0.007092843390004167,"score_gpt":0.1988399795399288,"score_spread":0.19174713614992464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097523063","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967609,0.0005826843,0.00041411349,0.000048225626,0.0000029641562,0.000004802247,0.00036062344,0.000026737696,0.0017990198],"genre_scores_gemma":[0.9978301,0.0001953602,0.00033412676,0.000039172814,0.00001604564,0.0000055465425,0.0011873234,0.000007679863,0.00038454455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995528,0.000048660255,0.000034019806,0.00007919329,0.000119393364,0.00016587893],"domain_scores_gemma":[0.99697053,0.0007871386,0.0013465917,0.00025231688,0.00024246963,0.00040093047],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006815286,0.00052064576,0.0003489441,0.00232145,0.0006451338,0.0018333426,0.0006090756,0.000660887,0.0015307611],"category_scores_gemma":[0.0022588237,0.00039527644,0.00030637567,0.0010055365,0.00054649287,0.0006700822,0.00076370593,0.00043771352,0.0005867687],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035572096,0.00011705758,0.917323,0.00009564153,0.00009686624,0.00072576065,0.00049226894,0.0006093294,0.0655868,0.00045157527,0.00040214704,0.013743857],"study_design_scores_gemma":[0.000009979204,0.000037443166,0.9955409,0.000011063346,0.000028049466,0.00031870854,0.00008145569,0.0002664477,0.0024108624,0.0001551698,0.0011304038,0.0000094905645],"about_ca_topic_score_codex":0.00441297,"about_ca_topic_score_gemma":0.010617997,"teacher_disagreement_score":0.00441297,"about_ca_system_score_codex":0.0006931399,"about_ca_system_score_gemma":0.00016403022,"threshold_uncertainty_score":0.008774579},"labels":[],"label_agreement":null},{"id":"W2097609835","doi":"10.1086/587687","title":"The<i>Spitzer</i>Survey of Interstellar Clouds in the Gould Belt. I. IC 5146 Observed With IRAC and MIPS","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Young stellar object; Spitzer Space Telescope; Star formation; Astronomy; Population; Spectral energy distribution; Line (geometry); Protostar; Telescope; Stars; Galaxy","score_opus":0.0329535736168878,"score_gpt":0.23519747324098875,"score_spread":0.20224389962410094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097609835","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90668285,0.0011673855,0.0004514559,0.0005780717,0.000054008164,0.00013354802,0.07590704,0.00082078314,0.014204839],"genre_scores_gemma":[0.8604209,0.0018115902,0.0039652986,0.0005021746,0.00013918166,0.00008877199,0.12377442,0.00011448225,0.00918324],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987626,0.000005547066,0.0000077581,0.000024325413,0.000039030216,0.000047156675],"domain_scores_gemma":[0.999701,0.000011023131,0.00013690404,0.000028878334,0.000034775934,0.00008739642],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013062087,0.00034694272,0.00020365228,0.0043455763,0.00029267216,0.00043298592,0.00044174894,0.00019707187,0.004632219],"category_scores_gemma":[0.00034229085,0.000112010326,0.00021977142,0.0021869233,0.00022537271,0.00037706847,0.00063586625,0.00020479746,0.0014439423],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013027494,0.00011840264,0.8664011,0.00015729813,0.000085026244,0.00044230017,0.00056906027,0.00030879618,0.012935148,0.0007203237,0.0635768,0.054555487],"study_design_scores_gemma":[0.0000053908757,0.000014354803,0.9828993,0.0000139789345,0.000007887861,0.00014491507,0.00009304411,0.00013419297,0.0004240584,0.00005789567,0.0162017,0.0000033754357],"about_ca_topic_score_codex":0.0357008,"about_ca_topic_score_gemma":0.09955399,"teacher_disagreement_score":0.0357008,"about_ca_system_score_codex":0.00061315385,"about_ca_system_score_gemma":0.0002739501,"threshold_uncertainty_score":0.07098597},"labels":[],"label_agreement":null},{"id":"W2097611961","doi":"10.1086/308761","title":"The Peculiar Type Ic Supernova 1997ef: Another Hypernova","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":195,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Hypernova; Light curve; Supernova; Physics; Astrophysics; Spectral line; Pair-instability supernova; Line (geometry); Kinetic energy; Astronomy; Ejecta; Geometry","score_opus":0.01056710319948789,"score_gpt":0.22448650757170432,"score_spread":0.21391940437221643,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097611961","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9867796,0.00041246865,0.005323103,0.0000914856,0.00002945972,0.000025192658,0.0005701036,0.00009761401,0.0066710855],"genre_scores_gemma":[0.9930768,0.0002956763,0.0027834913,0.00008168249,0.000024318571,0.000013735158,0.0016175687,0.000027050606,0.0020797148],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998807,0.000016618713,0.000011440898,0.000036399964,0.000023670667,0.00003108185],"domain_scores_gemma":[0.9997025,0.00004659683,0.00006647955,0.00005327212,0.000035894373,0.00009521739],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032475026,0.000409686,0.00031260925,0.0006562477,0.00033256147,0.0008847585,0.00034958703,0.000528971,0.0016596422],"category_scores_gemma":[0.00041982275,0.00010515868,0.00039658253,0.00077350286,0.00028132615,0.00046298365,0.00044617435,0.00048634235,0.00018454],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090082147,0.00034607184,0.7167895,0.00031190593,0.0004679401,0.01898922,0.0003755163,0.027871976,0.08431289,0.05340745,0.00456468,0.091661975],"study_design_scores_gemma":[0.00016895514,0.0006290474,0.7707225,0.00009897026,0.0001335647,0.053312793,0.00037696204,0.06510175,0.021737596,0.021092573,0.066477135,0.00014807603],"about_ca_topic_score_codex":0.0037730488,"about_ca_topic_score_gemma":0.003430473,"teacher_disagreement_score":0.0037730488,"about_ca_system_score_codex":0.00041388487,"about_ca_system_score_gemma":0.0001847858,"threshold_uncertainty_score":0.007502198},"labels":[],"label_agreement":null},{"id":"W2097815762","doi":"10.1086/588544","title":"The Balloon‐borne Large Aperture Submillimeter Telescope (BLAST) 2005: A 4 deg<sup>2</sup>Galactic Plane Survey in Vulpecula (ℓ = 59°)","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Galaxy; Astronomy; Molecular cloud; Telescope; Photometry (optics); Stars; Submillimeter Array; Protostar; Luminosity; Star formation","score_opus":0.013730246780188835,"score_gpt":0.22559389105655564,"score_spread":0.2118636442763668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097815762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98520976,0.00024455364,0.0007678116,0.000079277284,0.0000068519944,0.000029439458,0.009955575,0.00011964635,0.003587091],"genre_scores_gemma":[0.9566736,0.0004974887,0.0060103927,0.00012751602,0.00004241376,0.000040168303,0.033897076,0.000054411394,0.0026568891],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998752,0.00001029382,0.000006458643,0.00003183376,0.00004011661,0.00003611919],"domain_scores_gemma":[0.99962604,0.000021908536,0.00013607039,0.000040684503,0.000059763974,0.000115396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017958258,0.00022775626,0.00017914153,0.00097069476,0.00027809697,0.00044190537,0.0003537585,0.00019690057,0.0017769142],"category_scores_gemma":[0.00026561876,0.0001137672,0.00016459647,0.0009869834,0.0001209452,0.00017477066,0.0005006166,0.00020033488,0.00068706303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021331568,0.00006962895,0.9067656,0.000068041554,0.00009865936,0.00030983778,0.0004121445,0.00079099624,0.02793254,0.00036490863,0.009303604,0.05367074],"study_design_scores_gemma":[0.000011391204,0.000029898754,0.9901426,0.000008938347,0.00001739033,0.00020479319,0.00012690699,0.00037091144,0.0012389108,0.000051378393,0.007793501,0.0000034401623],"about_ca_topic_score_codex":0.030004743,"about_ca_topic_score_gemma":0.077820286,"teacher_disagreement_score":0.030004743,"about_ca_system_score_codex":0.00055512163,"about_ca_system_score_gemma":0.00041695393,"threshold_uncertainty_score":0.059660196},"labels":[],"label_agreement":null},{"id":"W2097937279","doi":"10.1088/0004-637x/804/1/33","title":"OGLE-2011-BLG-0265Lb: A JOVIAN MICROLENSING PLANET ORBITING AN M DWARF","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of British Columbia","funders":"Planning and Budgeting Committee of the Council for Higher Education of Israel; Japan Society for the Promotion of Science; Israeli Centers for Research Excellence; National Research Foundation of Korea; Fonds National de la Recherche Luxembourg; Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture; Ministerstwo Edukacji i Nauki; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; California Institute of Technology; European Commission; Fédération Wallonie-Bruxelles; National Aeronautics and Space Administration; Qatar National Research Fund; Qatar Foundation; Ohio State University; National Science Foundation","keywords":"Physics; Gravitational microlensing; Planet; Planetary system; Astrophysics; Astronomy; Brown dwarf; Exoplanet; Light curve; Jovian; Jupiter (rocket family); Bulge; Mass ratio; Jupiter mass; Planetary mass; Stars; Saturn","score_opus":0.02249047006948922,"score_gpt":0.23803521906986977,"score_spread":0.21554474900038056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097937279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9496996,0.0006754017,0.0011965417,0.0015581844,0.00034810955,0.00003626617,0.003815299,0.0006694883,0.042001087],"genre_scores_gemma":[0.9758263,0.00015686461,0.002342557,0.00075027754,0.000063495914,0.000009208707,0.004997669,0.00009791811,0.015755601],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999274,0.000005753821,0.0000025275115,0.000020661659,0.000021317917,0.000022371902],"domain_scores_gemma":[0.9997925,0.000015044135,0.000029417368,0.00001821007,0.000022454464,0.00012245507],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015569749,0.00015586193,0.0001589795,0.0005353742,0.0011386507,0.000670448,0.00023998322,0.0009565395,0.002421667],"category_scores_gemma":[0.00031908278,0.0000740607,0.000084304986,0.00068217324,0.00029997248,0.0006137862,0.0008074589,0.0004825302,0.0012154545],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022161761,0.000800004,0.33754697,0.00075074047,0.00014561445,0.049000185,0.008954687,0.0024290725,0.26252297,0.021328675,0.12058826,0.19371666],"study_design_scores_gemma":[0.00009636751,0.00064654916,0.58004683,0.00014839202,0.000049618753,0.01296063,0.0057614264,0.0045817913,0.013720236,0.0034464868,0.37845883,0.0000829232],"about_ca_topic_score_codex":0.010464518,"about_ca_topic_score_gemma":0.025009882,"teacher_disagreement_score":0.010464518,"about_ca_system_score_codex":0.0007009789,"about_ca_system_score_gemma":0.0004592514,"threshold_uncertainty_score":0.020807207},"labels":[],"label_agreement":null},{"id":"W2097957977","doi":"10.1088/0004-637x/780/2/127","title":"DISCOVERY OF THE THIRD TRANSIENT X-RAY BINARY IN THE GALACTIC GLOBULAR CLUSTER TERZAN 5","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"RIKEN; Natural Sciences and Engineering Research Council of Canada; Japan Aerospace Exploration Agency; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution","keywords":"Globular cluster; Astrophysics; Physics; Acis; Neutron star; Swift; Luminosity; Accretion (finance); Astronomy; Galaxy","score_opus":0.008917593842949115,"score_gpt":0.213622179309177,"score_spread":0.20470458546622788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097957977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99940073,0.00007758956,0.000085283595,0.000011579055,0.000005026516,0.0000042407187,0.000044936067,0.0000053353206,0.00036525383],"genre_scores_gemma":[0.99896896,0.00005647205,0.0002942622,0.00002349579,0.000006791853,0.0000035917922,0.00033507388,0.0000029836071,0.00030828736],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991465,0.0000037407767,0.000003860626,0.000031458094,0.000022529197,0.000023839502],"domain_scores_gemma":[0.99975246,0.000014740384,0.000087870954,0.000024104967,0.000022182536,0.00009865202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000113617265,0.00018426219,0.00019994595,0.0005587984,0.0005904104,0.000759853,0.00028922045,0.000378377,0.00051233044],"category_scores_gemma":[0.0002404502,0.00014582767,0.00025972966,0.00040706096,0.00028933847,0.00019663358,0.00077698386,0.00034871197,0.00019534102],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052786514,0.00013507194,0.86446637,0.00007310947,0.0000883302,0.006352658,0.0014667257,0.00033952517,0.11037247,0.0006641541,0.00041311068,0.015100488],"study_design_scores_gemma":[0.000015564498,0.00025047033,0.99096745,0.000011238317,0.000029551613,0.0023440518,0.00035731343,0.000508705,0.0031857009,0.00008092228,0.0022364473,0.0000124985445],"about_ca_topic_score_codex":0.0036450652,"about_ca_topic_score_gemma":0.007727746,"teacher_disagreement_score":0.0036450652,"about_ca_system_score_codex":0.0003623734,"about_ca_system_score_gemma":0.00017994785,"threshold_uncertainty_score":0.0072476864},"labels":[],"label_agreement":null},{"id":"W2097986782","doi":"10.1088/0004-637x/740/2/69","title":"A BAYESIAN APPROACH TO LOCATING THE RED GIANT BRANCH TIP MAGNITUDE. I.","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Andromeda; Red-giant branch; Bayesian probability; Algorithm; Population; Prior probability; Computer science; Magnitude (astronomy); Local Group; Astrophysics; Galaxy; Mathematics; Artificial intelligence; Physics; Milky Way; Metallicity","score_opus":0.02084794617849331,"score_gpt":0.2170200156572906,"score_spread":0.19617206947879728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2097986782","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.002073884,0.00034444226,0.9948143,0.00027766786,0.000037584858,0.000036313053,0.00014991019,0.00026472547,0.0020012802],"genre_scores_gemma":[0.058580246,0.0006759461,0.93558586,0.00020675972,0.00018356001,0.00018558935,0.0004281261,0.00018693673,0.003966914],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9990989,0.0002913398,0.000054250835,0.00022352673,0.00026934766,0.00006281083],"domain_scores_gemma":[0.99870205,0.0005443289,0.00019984848,0.00012979051,0.0003441361,0.000079773185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00209807,0.0008013705,0.00081838074,0.0027348916,0.001021475,0.0022867087,0.001952139,0.0014126821,0.0034698595],"category_scores_gemma":[0.0061457846,0.0009023998,0.00083487347,0.001553071,0.0010266036,0.0017775097,0.0022276274,0.0016263556,0.0019837723],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000088718945,0.00009746844,0.008049932,0.00028185494,0.00021853653,0.00017897501,0.00040767188,0.23486413,0.007925006,0.14165065,0.011133032,0.59510404],"study_design_scores_gemma":[0.000030297959,0.000041323874,0.0034503788,0.00012503997,0.0000549463,0.00037195638,0.000116310104,0.8050216,0.0023171166,0.16444498,0.023942217,0.00008383018],"about_ca_topic_score_codex":0.008814375,"about_ca_topic_score_gemma":0.011962834,"teacher_disagreement_score":0.008814375,"about_ca_system_score_codex":0.0015123974,"about_ca_system_score_gemma":0.002162934,"threshold_uncertainty_score":0.01752609},"labels":[],"label_agreement":null},{"id":"W2098397848","doi":"10.1086/317103","title":"Discovery of a Young Radio Pulsar in a Relativistic Binary Orbit","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Neutron star; White dwarf; Orbit (dynamics); X-ray pulsar; Binary pulsar; Astronomy; Binary number; Roche lobe; Millisecond pulsar; Orbital period; Stars","score_opus":0.009218048493443261,"score_gpt":0.2882984020233277,"score_spread":0.2790803535298844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2098397848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982817,0.0006336296,0.00042389208,0.00005884763,0.000027747197,0.0000061209507,0.000016255583,0.000014166246,0.00053766166],"genre_scores_gemma":[0.99845123,0.00028111876,0.0007234701,0.00008870039,0.000043964596,0.0000033306592,0.00008477486,0.0000025857694,0.0003208258],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998493,0.000018037517,0.000016163793,0.00004491047,0.000030669773,0.00004090058],"domain_scores_gemma":[0.9995956,0.000060166578,0.00017673436,0.00004798545,0.00002294244,0.00009656163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003831451,0.00027259556,0.00030107587,0.00067935325,0.0007737332,0.001058014,0.00050409924,0.00090772304,0.0004811181],"category_scores_gemma":[0.0008413707,0.00028604243,0.000270912,0.00039583378,0.0005924756,0.0005027228,0.0009234943,0.00041108025,0.0003453584],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010079165,0.0003522876,0.68606704,0.00028175832,0.00018162475,0.07181467,0.0028744268,0.000468472,0.14967299,0.00340801,0.0010515981,0.08281921],"study_design_scores_gemma":[0.00014709252,0.0037660636,0.81075644,0.00006651632,0.0004415937,0.12689331,0.0009377938,0.0015475784,0.031416077,0.0018716737,0.022073263,0.00008263804],"about_ca_topic_score_codex":0.000485388,"about_ca_topic_score_gemma":0.0007124311,"teacher_disagreement_score":0.001058014,"about_ca_system_score_codex":0.00020433539,"about_ca_system_score_gemma":0.00014356742,"threshold_uncertainty_score":0.00202626},"labels":[],"label_agreement":null},{"id":"W2098446021","doi":"10.1088/0004-637x/766/1/49","title":"CHARACTERIZING MAGNETIZED TURBULENCE IN M51","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Western University","funders":"","keywords":"Physics; Turbulence; Faraday effect; Anisotropy; Magnetic field; Astrophysics; Optics; Mechanics","score_opus":0.00621687014823645,"score_gpt":0.19751230163936953,"score_spread":0.1912954314911331,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2098446021","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989166,0.000031543255,0.00039826415,0.0000111110485,0.000001573227,0.000003573694,0.00012944567,0.00001260646,0.0004951948],"genre_scores_gemma":[0.99880147,0.000029708974,0.0007152121,0.000009863362,0.0000039269908,0.000004916239,0.00034528764,0.0000033930573,0.00008619669],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990404,0.000010284324,0.000006883917,0.000028159156,0.000020772608,0.000029802588],"domain_scores_gemma":[0.99972624,0.000036756897,0.000095229276,0.00005953286,0.00004231205,0.000039907758],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019609007,0.00020440982,0.0001460648,0.0010561927,0.00035772627,0.00046429774,0.00019841979,0.00020583757,0.000365953],"category_scores_gemma":[0.00055236253,0.00018324947,0.00025824612,0.00066634343,0.00027192896,0.00023236402,0.00050587783,0.00013998375,0.00016867802],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026969463,0.00008078726,0.81584126,0.00003431108,0.000095927,0.0006163909,0.0008528609,0.006955941,0.15780295,0.0012025374,0.0004589227,0.01578845],"study_design_scores_gemma":[0.000013062285,0.00006451563,0.9875672,0.0000073929555,0.000015725229,0.00014809267,0.00010187137,0.006491733,0.004724893,0.00018110583,0.000667846,0.000016544558],"about_ca_topic_score_codex":0.003416394,"about_ca_topic_score_gemma":0.0070066513,"teacher_disagreement_score":0.003416394,"about_ca_system_score_codex":0.00038293476,"about_ca_system_score_gemma":0.00016192177,"threshold_uncertainty_score":0.006793022},"labels":[],"label_agreement":null},{"id":"W2098472138","doi":"10.1086/318176","title":"Discovery of an Extremely Metal-Poor Galaxy: Optical Spectroscopy of UGCA 292","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Metallicity; Galaxy; Dwarf galaxy; Irregular galaxy; Spectroscopy; Abundance (ecology); Galaxy group; Astronomy; Elliptical galaxy; Interacting galaxy; Biology","score_opus":0.01102573549112212,"score_gpt":0.23459539433118726,"score_spread":0.22356965884006513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2098472138","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979063,0.000047996044,0.00010774781,0.000031915686,0.000003988314,0.000008298134,0.00013605709,0.00001623215,0.001741436],"genre_scores_gemma":[0.99871624,0.000021490672,0.0003044348,0.000045582223,0.000005216972,0.0000044457256,0.00043597026,0.00000619802,0.0004603648],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984336,0.000009469064,0.000004700554,0.000040299426,0.000044041306,0.00005812034],"domain_scores_gemma":[0.9995653,0.000016801114,0.000050037273,0.000041505464,0.00006408714,0.0002621958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111361216,0.00030647588,0.00040374338,0.0009972982,0.0012696232,0.0009845003,0.0004149151,0.0005901328,0.00085998164],"category_scores_gemma":[0.00037167553,0.00022339378,0.00025644712,0.00060655334,0.00052371406,0.00017356731,0.00073678896,0.00039638867,0.00033022134],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003584448,0.00024942568,0.77297676,0.000041713596,0.00008259064,0.0044066454,0.00097369176,0.00033840336,0.20818894,0.0007689775,0.0016402326,0.009974159],"study_design_scores_gemma":[0.000013780476,0.000067922185,0.99238,0.0000032688702,0.000016665443,0.0011511747,0.00020003463,0.00042699842,0.0032531715,0.000085656495,0.002391298,0.000009988738],"about_ca_topic_score_codex":0.026512563,"about_ca_topic_score_gemma":0.04451947,"teacher_disagreement_score":0.026512563,"about_ca_system_score_codex":0.0005810864,"about_ca_system_score_gemma":0.00029544093,"threshold_uncertainty_score":0.052716494},"labels":[],"label_agreement":null},{"id":"W2098517949","doi":"10.1088/0004-637x/746/1/21","title":"EARLY RADIO AND X-RAY OBSERVATIONS OF THE YOUNGEST NEARBY TYPE Ia SUPERNOVA PTF 11kly (SN 2011fe)","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":142,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; University of Oxford; University of Leicester; Weizmann Institute of Science; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Supernova; Physics; Astrophysics; Context (archaeology); White dwarf; Astronomy; Stars; Red giant; Type (biology); Geology","score_opus":0.02095344226071529,"score_gpt":0.23591619698308258,"score_spread":0.21496275472236728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2098517949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99025947,0.0004899903,0.0016263452,0.00015220052,0.000022007303,0.000019543408,0.0013201009,0.0000802896,0.006029967],"genre_scores_gemma":[0.9938253,0.0005767052,0.0015852748,0.000087266744,0.00004716567,0.000010466841,0.002149234,0.000016175747,0.001702501],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968505,0.000025804497,0.000023107079,0.000110277135,0.00007393003,0.00008182723],"domain_scores_gemma":[0.9988255,0.0002985766,0.00047268425,0.00012651454,0.00010171557,0.00017506206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005671808,0.0003267714,0.00031566343,0.0011789073,0.0006521593,0.0015824506,0.00038191435,0.00044360565,0.0013378017],"category_scores_gemma":[0.0016390972,0.00024369502,0.00032302632,0.0005851458,0.00059005455,0.00043687856,0.00096765364,0.00047493193,0.00054528937],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019358312,0.00006269471,0.9632292,0.000096940516,0.00007747834,0.0011785818,0.00050054054,0.0013829954,0.009967225,0.0015916084,0.001188102,0.020531032],"study_design_scores_gemma":[0.000004444163,0.0000552242,0.99041265,0.000026359727,0.000019317604,0.00064534,0.00013076125,0.00087491993,0.0034390436,0.00026563773,0.0041104285,0.000015850543],"about_ca_topic_score_codex":0.0069302316,"about_ca_topic_score_gemma":0.020523546,"teacher_disagreement_score":0.0069302316,"about_ca_system_score_codex":0.00067209755,"about_ca_system_score_gemma":0.0002630908,"threshold_uncertainty_score":0.013779759},"labels":[],"label_agreement":null},{"id":"W2098672383","doi":"10.1088/0004-637x/763/2/147","title":"COSMOLOGICAL CONSTRAINTS FROM SUNYAEV–ZEL'DOVICH-SELECTED CLUSTERS WITH X-RAY OBSERVATIONS IN THE FIRST 178 deg<sup>2</sup> OF THE SOUTH POLE TELESCOPE SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":255,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"University of Chicago; McGill University; Gordon and Betty Moore Foundation; Jet Propulsion Laboratory; Deutsche Forschungsgemeinschaft; Smithsonian Astrophysical Observatory; Massachusetts Institute of Technology; Kavli Institute for Cosmological Physics, University of Chicago; Canada Research Chairs; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; South Pole Telescope; Astrophysics; Cosmic microwave background; Galaxy cluster; Sunyaev–Zel'dovich effect; CMB cold spot; Cluster (spacecraft); Omega; Dark energy; Cosmology; Observable; Sigma; Galaxy; Astronomy","score_opus":0.015128344878675901,"score_gpt":0.19747957050206766,"score_spread":0.18235122562339176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2098672383","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99771786,0.0002049866,0.000036594407,0.00017455769,0.0000069310627,0.0000022626286,0.000701248,0.0000032707567,0.0011523225],"genre_scores_gemma":[0.99815947,0.00006872755,0.00006786579,0.000031530864,0.000014307675,0.0000023108137,0.0012581812,0.000007822767,0.00038980244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999493,0.00008749664,0.000025457684,0.00018528465,0.000078671954,0.00013006176],"domain_scores_gemma":[0.9972415,0.00045294364,0.00090379163,0.00018848773,0.00023351479,0.0009796892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071800925,0.00023944405,0.0004074426,0.0015324805,0.0012508396,0.0015047608,0.000661664,0.00041324814,0.0035728628],"category_scores_gemma":[0.0030765028,0.00031335762,0.00021452316,0.00208448,0.0007248206,0.00051874906,0.001990453,0.0005292617,0.00041430825],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012235212,0.000021691816,0.9947529,0.000011440097,0.00006360506,0.00008665504,0.0006191254,0.00014151467,0.0005246327,0.0005069483,0.0011590801,0.0019900983],"study_design_scores_gemma":[0.0000047244494,0.000003364538,0.9984189,0.0000058271553,0.000012370382,0.000031163443,0.00046770432,0.00012201657,0.000033483015,0.00009774376,0.0007990752,0.000003485352],"about_ca_topic_score_codex":0.12318098,"about_ca_topic_score_gemma":0.2925145,"teacher_disagreement_score":0.12318098,"about_ca_system_score_codex":0.0009335588,"about_ca_system_score_gemma":0.00090534735,"threshold_uncertainty_score":0.244928},"labels":[],"label_agreement":null},{"id":"W2098921755","doi":"10.1086/587458","title":"Observation of Gamma‐Ray Emission from the Galaxy M87 above 250 GeV with VERITAS1","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Telescope; RADIUS; Astronomy; Observatory; Gamma ray; Radio galaxy","score_opus":0.013084992459338612,"score_gpt":0.20430526171091282,"score_spread":0.1912202692515742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2098921755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981742,0.0001546356,0.00021228722,0.000024580333,0.000002837289,0.0000024274311,0.00025351517,0.00005329934,0.0011221874],"genre_scores_gemma":[0.9975725,0.000107732405,0.00084484415,0.000030781284,0.00001001119,0.0000029236398,0.0008900563,0.000011190807,0.0005300242],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987686,0.000010184891,0.0000040504815,0.000023095823,0.000053950822,0.000031795396],"domain_scores_gemma":[0.9997203,0.000039002476,0.0001160574,0.00004071295,0.000034681318,0.000049218437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016268753,0.00014791799,0.00016394391,0.00064504746,0.0002975511,0.00037783652,0.00039910502,0.00023794475,0.00093367894],"category_scores_gemma":[0.00035653633,0.00013268416,0.00013059459,0.0004517447,0.00018534306,0.00018877929,0.00043766137,0.0002817524,0.00025177374],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041058654,0.00009507968,0.678094,0.00006229255,0.00010247411,0.001207777,0.0005055334,0.0007537549,0.28281268,0.0005929587,0.001997387,0.03336534],"study_design_scores_gemma":[0.000012009516,0.0001367054,0.9813421,0.00001049982,0.000026319774,0.0006014189,0.000072188675,0.0010164636,0.014390949,0.00006104627,0.0023246943,0.000005639068],"about_ca_topic_score_codex":0.0054412563,"about_ca_topic_score_gemma":0.014322248,"teacher_disagreement_score":0.0054412563,"about_ca_system_score_codex":0.00032214154,"about_ca_system_score_gemma":0.0001670741,"threshold_uncertainty_score":0.010819137},"labels":[],"label_agreement":null},{"id":"W2099045096","doi":"10.1088/0004-637x/790/1/51","title":"X- AND γ-RAY PULSATIONS OF THE NEARBY RADIO-FAINT PSR J1741–2054","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Pulsar; Physics; Astrophysics; Neutron star; Nebula; Fermi Gamma-ray Space Telescope; Pulsar wind nebula; Astronomy; Light curve; Black-body radiation; Binary pulsar; X-ray pulsar; Synchrotron radiation; Millisecond pulsar; Radiation; Optics; Stars","score_opus":0.00802382287463881,"score_gpt":0.2800617267017567,"score_spread":0.2720379038271179,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099045096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967409,0.0001852028,0.000132459,0.00007312269,0.000011295989,0.0000046434575,0.0002448424,0.000010932432,0.0025966817],"genre_scores_gemma":[0.9976597,0.00012286,0.00028986004,0.000049692502,0.000030386645,0.000007498226,0.00065683183,0.000007474786,0.0011757336],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996483,0.0000037725708,0.0000019529741,0.000012908438,0.000009232778,0.000007428481],"domain_scores_gemma":[0.9998429,0.000020391333,0.00007672401,0.00001660758,0.000011693822,0.000031614207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106866675,0.00021801786,0.0001539468,0.000660157,0.00043218094,0.00031487804,0.00013424427,0.00022894697,0.0030326636],"category_scores_gemma":[0.00028970724,0.00011754715,0.00013298994,0.0005745728,0.00041292503,0.00028895665,0.00043048424,0.0002641356,0.0005214737],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013780616,0.00016155784,0.76126707,0.000101021964,0.00011333436,0.0027104144,0.0007971636,0.00088526437,0.19512986,0.002532569,0.0015769637,0.033346716],"study_design_scores_gemma":[0.000021412976,0.000121729514,0.9958156,0.00000425738,0.00001209772,0.00066336145,0.000106204454,0.00015194077,0.0012947465,0.00037297574,0.0014294226,0.0000062458344],"about_ca_topic_score_codex":0.0013562869,"about_ca_topic_score_gemma":0.0016926249,"teacher_disagreement_score":0.0030326636,"about_ca_system_score_codex":0.00018098202,"about_ca_system_score_gemma":0.00010700688,"threshold_uncertainty_score":0.010145247},"labels":[],"label_agreement":null},{"id":"W2099217445","doi":"10.1086/308645","title":"The Absolute Flux of Protons and Helium at the Top of the Atmosphere Using IMAX","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":164,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Goddard Space Flight Center; Bundesministerium für Bildung und Forschung; Deutsche Forschungsgemeinschaft; New Mexico State University; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Atmosphere (unit); Helium; Flux (metallurgy); Nuclear physics; Atomic physics; Astrophysics; Astronomy; Meteorology","score_opus":0.006191204588365392,"score_gpt":0.2175855265485602,"score_spread":0.2113943219601948,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099217445","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9699808,0.0006247275,0.012810915,0.00009618376,0.00002106571,0.00002560236,0.0028539116,0.0008944154,0.012692395],"genre_scores_gemma":[0.978819,0.00033633635,0.017167136,0.00004324651,0.000025529558,0.000021012764,0.0021753893,0.00013059177,0.0012818022],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9996648,0.000052605676,0.000011553906,0.00013802279,0.000096966425,0.000035974543],"domain_scores_gemma":[0.9996972,0.000055378518,0.00008976519,0.000068818925,0.000057431153,0.000031488828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005688144,0.0005869248,0.00043752897,0.0010222178,0.00041303155,0.0004917882,0.0005050455,0.00030242366,0.0015444909],"category_scores_gemma":[0.0004926144,0.00025709663,0.00022387566,0.0010354498,0.00030290437,0.0005205671,0.00057805947,0.00029096723,0.00029444127],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0032398093,0.00008555233,0.21477695,0.0004627532,0.00037418256,0.0005185453,0.000759078,0.0042966674,0.70691544,0.003389768,0.001854957,0.0633263],"study_design_scores_gemma":[0.000097578326,0.00051306665,0.5762159,0.000053372474,0.00033957185,0.0009535029,0.00014454682,0.010658025,0.39490575,0.0006724844,0.015371629,0.00007458771],"about_ca_topic_score_codex":0.002402557,"about_ca_topic_score_gemma":0.0045552724,"teacher_disagreement_score":0.002402557,"about_ca_system_score_codex":0.0004977014,"about_ca_system_score_gemma":0.0001588048,"threshold_uncertainty_score":0.0051668882},"labels":[],"label_agreement":null},{"id":"W2099265861","doi":"10.1088/0004-637x/736/1/39","title":"THE ATACAMA COSMOLOGY TELESCOPE: DETECTION OF SUNYAEV-ZEL'DOVICH DECREMENT IN GROUPS AND CLUSTERS ASSOCIATED WITH LUMINOUS RED GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Sky; Halo; Luminosity; Galaxy; Cosmology; Galaxy cluster; Cluster (spacecraft); South Pole Telescope; Telescope","score_opus":0.009147591824726018,"score_gpt":0.19216720101425935,"score_spread":0.18301960918953333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099265861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9843321,0.0006068716,0.00040165277,0.00062080467,0.000060230996,0.000034984983,0.004799216,0.00007805294,0.009066188],"genre_scores_gemma":[0.9928756,0.00021708946,0.00095353724,0.00018410828,0.000035438137,0.000022275946,0.003184322,0.000017627051,0.0025100973],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998355,0.00001668418,0.000008767295,0.000050218427,0.000055298937,0.00003347822],"domain_scores_gemma":[0.9991393,0.00006275033,0.00024358109,0.000090460744,0.0001537145,0.000310128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054209505,0.000109622466,0.00016446153,0.0017264903,0.0007367553,0.0006643292,0.00034046228,0.00039378254,0.0022603248],"category_scores_gemma":[0.0010510425,0.00014465851,0.00011909363,0.0012348809,0.00039058022,0.00031909466,0.00081086584,0.00045448917,0.00034036476],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012086071,0.000038217207,0.9755265,0.000043305274,0.000057050067,0.00022612767,0.0005459553,0.000038416838,0.0057898266,0.0005028674,0.0050208424,0.012089945],"study_design_scores_gemma":[0.000004410264,0.0000050737676,0.998114,0.0000039706974,0.000005199094,0.0000697726,0.000092521695,0.000033662367,0.00013483295,0.000044068147,0.0014907793,0.0000017086129],"about_ca_topic_score_codex":0.039411124,"about_ca_topic_score_gemma":0.08565359,"teacher_disagreement_score":0.039411124,"about_ca_system_score_codex":0.00049923133,"about_ca_system_score_gemma":0.0006190166,"threshold_uncertainty_score":0.07836348},"labels":[],"label_agreement":null},{"id":"W2099295799","doi":"10.1088/0004-637x/754/1/77","title":"VERITAS OBSERVATIONS OF THE NOVA IN V407 CYGNI","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Zenith; Nova (rocket); Astrophysics; Fermi Gamma-ray Space Telescope; Telescope; Flux (metallurgy); Astronomy; Radiation; Optics","score_opus":0.034176995570540644,"score_gpt":0.25167474949554386,"score_spread":0.2174977539250032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099295799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933194,0.00031273754,0.00025878704,0.00005325004,0.000012210154,0.000012086572,0.00042293698,0.000032993365,0.005575676],"genre_scores_gemma":[0.9966378,0.0001642753,0.00081241515,0.000048668033,0.000017238059,0.000011907862,0.0011282226,0.000014302085,0.0011651285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999821,0.000012932369,0.0000051025754,0.000040994506,0.000071094124,0.00004892877],"domain_scores_gemma":[0.9997634,0.00003230217,0.000070958486,0.000028339213,0.000033100947,0.000071931034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002630233,0.00023320077,0.00022889131,0.0007666332,0.0005640389,0.00051624916,0.00032122488,0.00039187213,0.00090311025],"category_scores_gemma":[0.0004707434,0.00021013139,0.00017911557,0.00042178854,0.00035960428,0.00022044069,0.0009031219,0.00034795864,0.0003466617],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010309684,0.00014214324,0.6859409,0.00016510651,0.00021425911,0.0038817876,0.0013148157,0.00195366,0.25304163,0.0025332852,0.0032658156,0.04651559],"study_design_scores_gemma":[0.0000296224,0.00025329206,0.9817104,0.00003355624,0.000039123315,0.0012362534,0.0001916304,0.0011566739,0.0071223313,0.00044967426,0.007760133,0.000017510318],"about_ca_topic_score_codex":0.0071822116,"about_ca_topic_score_gemma":0.021742841,"teacher_disagreement_score":0.0071822116,"about_ca_system_score_codex":0.0006055526,"about_ca_system_score_gemma":0.00030545754,"threshold_uncertainty_score":0.014280796},"labels":[],"label_agreement":null},{"id":"W2099312297","doi":"10.1088/0004-637x/718/1/306","title":"AN OBSERVED LACK OF SUBSTRUCTURE IN STARLESS CORES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Substructure; Astrophysics; Bolometer; Physics; Core (optical fiber); Resolution (logic); Astronomy; Optics; Detector","score_opus":0.027058284192388177,"score_gpt":0.2784719515717076,"score_spread":0.25141366737931947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099312297","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981762,0.00012384576,0.00068712817,0.000014480715,0.0000040322398,0.0000029100026,0.00016708524,0.000026429365,0.0007978527],"genre_scores_gemma":[0.99927944,0.00002383254,0.00032601156,0.000017770293,0.000004021258,0.0000013846375,0.00019915235,0.0000034830637,0.00014484374],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986446,0.000009272422,0.000010276653,0.000055665158,0.00003884439,0.000021515956],"domain_scores_gemma":[0.99907035,0.00013816376,0.0003668211,0.000115346804,0.00016676969,0.0001426488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021894423,0.00016844575,0.00019715268,0.0007208477,0.00025183737,0.00050279254,0.00030002766,0.0001586866,0.0017387832],"category_scores_gemma":[0.0007344385,0.00010236191,0.00011503819,0.00036169004,0.00049935083,0.00023769714,0.0005217315,0.00013520932,0.00030364777],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030054172,0.000030218262,0.8865996,0.00006726598,0.000074667274,0.0003719937,0.00036306123,0.00022552662,0.099672146,0.0003565412,0.00019771211,0.011740741],"study_design_scores_gemma":[0.000009936171,0.00007188478,0.9900141,0.0000048630372,0.000014210692,0.0007177945,0.000113802846,0.0002526638,0.007901868,0.00026623573,0.0006288655,0.0000037817606],"about_ca_topic_score_codex":0.0014278283,"about_ca_topic_score_gemma":0.0025786958,"teacher_disagreement_score":0.0017387832,"about_ca_system_score_codex":0.0001465865,"about_ca_system_score_gemma":0.00010429386,"threshold_uncertainty_score":0.0058168173},"labels":[],"label_agreement":null},{"id":"W2099351385","doi":"10.1088/0004-637x/809/2/168","title":"BROADBAND SPECTRAL MODELING OF THE EXTREME GIGAHERTZ-PEAKED SPECTRUM RADIO SOURCE PKS B0008-421","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"U.S. Air Force; Ministero dello Sviluppo Economico; Jet Propulsion Laboratory; Victoria University; Smithsonian Astrophysical Observatory; Astronomy Australia Limited; Victoria University of Wellington; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Harvard University; Curtin University of Technology; California Institute of Technology; National Aeronautics and Space Administration; Nvidia; Smithsonian Institution; National Science Foundation","keywords":"Physics; Absorption (acoustics); Broadband; Computational physics; Synchrotron; Radio spectrum; Spectral slope; Spectral line; Optics; Astronomy","score_opus":0.027150805118981998,"score_gpt":0.2160611366967412,"score_spread":0.18891033157775922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099351385","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96771866,0.00012715082,0.025952011,0.00012598986,0.0000075764106,0.000032756994,0.000659658,0.00042172577,0.004954395],"genre_scores_gemma":[0.99430674,0.000057316774,0.0042943456,0.000027198748,0.00000724057,0.000026411659,0.00068794965,0.000054926953,0.00053789595],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999095,0.000015768475,0.0000035206542,0.00003117698,0.000019897569,0.000020029393],"domain_scores_gemma":[0.99984527,0.000027561451,0.000050565846,0.000024552406,0.000020221758,0.000031834385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024264383,0.00037530242,0.00020367403,0.0005785231,0.00033971254,0.0004672748,0.0007238028,0.00052055274,0.00093518704],"category_scores_gemma":[0.00046808037,0.00032492122,0.00040872695,0.0004115651,0.00020790589,0.0003899143,0.0004099831,0.00039418705,0.0003948407],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005737717,0.00027281002,0.2765148,0.00013149098,0.00014366841,0.0009567076,0.0006352791,0.5198723,0.1567307,0.015351892,0.0020354888,0.026781097],"study_design_scores_gemma":[0.00008057696,0.0001598427,0.28031096,0.000027488311,0.000054935612,0.00043225702,0.00016098164,0.7051977,0.0054177586,0.0046774806,0.0033996052,0.00008036208],"about_ca_topic_score_codex":0.0032908423,"about_ca_topic_score_gemma":0.0026792318,"teacher_disagreement_score":0.0032908423,"about_ca_system_score_codex":0.00057206873,"about_ca_system_score_gemma":0.00016302637,"threshold_uncertainty_score":0.0065433383},"labels":[],"label_agreement":null},{"id":"W2099369883","doi":"10.1088/0004-637x/752/2/146","title":"MILKY WAY STAR-FORMING COMPLEXES AND THE TURBULENT MOTION OF THE GALAXY'S MOLECULAR GAS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Milky Way; Luminosity; CMB cold spot; Proper motion; Turbulence; Flux (metallurgy); Luminosity function; Molecular cloud; Kinetic energy","score_opus":0.009480945198548807,"score_gpt":0.2231514338946446,"score_spread":0.21367048869609578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099369883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99945647,0.00010682793,0.00008897244,0.0000056303197,3.2283415e-7,0.0000014934677,0.00008820936,0.000004462334,0.00024760855],"genre_scores_gemma":[0.99906737,0.0001049817,0.00028396034,0.0000043891255,0.000003077,0.0000022484694,0.00040921726,0.000003353473,0.00012150167],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989665,0.00000875144,0.000008725573,0.000030199053,0.000025706468,0.000029914301],"domain_scores_gemma":[0.99946386,0.000069778194,0.00031349517,0.00003969439,0.000034134027,0.000079110236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001761452,0.0002422795,0.0002067814,0.0019105852,0.0001935757,0.00075602386,0.00023274007,0.00015992473,0.0006871527],"category_scores_gemma":[0.00077932,0.0001494071,0.00024458187,0.001514397,0.00027680266,0.00041914717,0.0005274686,0.00011682572,0.00014733845],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004675013,0.0000130545095,0.9889712,0.000021162621,0.00006395283,0.00012417376,0.00032216057,0.0007766869,0.0028866779,0.000387704,0.000114347,0.006272156],"study_design_scores_gemma":[0.0000023064624,0.000010876411,0.9980944,0.000003887917,0.000013163459,0.00007210308,0.000091453585,0.0009168396,0.00034961637,0.00009797811,0.00034507195,0.0000023552889],"about_ca_topic_score_codex":0.0075645046,"about_ca_topic_score_gemma":0.008863137,"teacher_disagreement_score":0.0075645046,"about_ca_system_score_codex":0.0003565535,"about_ca_system_score_gemma":0.00014172493,"threshold_uncertainty_score":0.015040994},"labels":[],"label_agreement":null},{"id":"W2099378658","doi":"10.1086/518401","title":"Improved Measurements of the CMB Power Spectrum with ACBAR","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; CMB cold spot; Astrophysics; Anisotropy; Spectral density; Multipole expansion; Cosmology; Cosmic variance; Computational physics; Optics","score_opus":0.007841375978627588,"score_gpt":0.2311759772641159,"score_spread":0.22333460128548832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099378658","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87463903,0.0021062833,0.0926582,0.00029860102,0.00032723584,0.000087990964,0.006336628,0.005046857,0.018499201],"genre_scores_gemma":[0.93037915,0.00034354415,0.06151608,0.00011932434,0.00017129857,0.0000576224,0.0058413893,0.0003701881,0.0012014838],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983217,0.00025791102,0.000056140645,0.0005134654,0.000689978,0.00016068168],"domain_scores_gemma":[0.99849427,0.00023194835,0.00031293667,0.0005032658,0.0003367402,0.00012080604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015284357,0.00076776964,0.00048904435,0.001700946,0.00023599424,0.00094039534,0.0007977266,0.00041147586,0.0024046127],"category_scores_gemma":[0.0017466597,0.00046413872,0.00034619236,0.002114542,0.00019636641,0.000890912,0.0007890354,0.00093019113,0.001045608],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016815295,0.0005708107,0.39358458,0.00046091437,0.0006163436,0.00038895925,0.0006607632,0.020311344,0.33944985,0.0047021382,0.007033081,0.23053968],"study_design_scores_gemma":[0.00032953365,0.00050224265,0.7136501,0.00007709276,0.00032062622,0.0007809249,0.00010646423,0.056067917,0.1696515,0.0022909152,0.055995125,0.00022757507],"about_ca_topic_score_codex":0.0015445587,"about_ca_topic_score_gemma":0.0037489734,"teacher_disagreement_score":0.0024046127,"about_ca_system_score_codex":0.00040749018,"about_ca_system_score_gemma":0.00019619463,"threshold_uncertainty_score":0.008083284},"labels":[],"label_agreement":null},{"id":"W2099424148","doi":"10.1086/522204","title":"Quantifying Resonant Structure in NGC 6946 from Two-dimensional Kinematics","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; RADIUS; Kinematics; Galaxy; Astrophysics; Perturbation (astronomy); Resonance (particle physics); Geometry; Classical mechanics; Astronomy; Atomic physics; Mathematics","score_opus":0.01344438197455693,"score_gpt":0.24950258592982472,"score_spread":0.23605820395526778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099424148","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985734,0.000053078144,0.0007324183,0.000005617164,0.0000010377855,0.0000022626823,0.00008788794,0.00002524218,0.00051903265],"genre_scores_gemma":[0.9989027,0.000037009195,0.00085155055,0.000001935965,0.0000015084515,0.0000012336245,0.00012743301,0.000005333089,0.00007128778],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991906,0.000011607843,0.0000046545774,0.000023406305,0.000019083822,0.000022193595],"domain_scores_gemma":[0.9996965,0.000035735877,0.0001415549,0.000035961857,0.000024093599,0.00006619522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012014484,0.00022491117,0.00015361761,0.00081738975,0.00022423861,0.0005355919,0.00021231834,0.00020144372,0.0005023638],"category_scores_gemma":[0.0005722934,0.00016728723,0.00021821252,0.00045477826,0.00020534867,0.00022692216,0.0004254038,0.0001022083,0.00022086396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031420187,0.00006351906,0.73567766,0.000058939466,0.00011563538,0.0015362308,0.0011624529,0.032629516,0.20365536,0.002637959,0.0002560951,0.02189246],"study_design_scores_gemma":[0.000016334368,0.000085463624,0.9505759,0.000009855785,0.000032508695,0.00081509363,0.00028726726,0.03916728,0.0074454565,0.00076459977,0.0007669166,0.000033400822],"about_ca_topic_score_codex":0.009096295,"about_ca_topic_score_gemma":0.010501328,"teacher_disagreement_score":0.009096295,"about_ca_system_score_codex":0.0003238061,"about_ca_system_score_gemma":0.00015607772,"threshold_uncertainty_score":0.018086672},"labels":[],"label_agreement":null},{"id":"W2099526242","doi":"10.1088/0004-637x/747/2/116","title":"INFRARED NON-DETECTION OF FOMALHAUT b: IMPLICATIONS FOR THE PLANET INTERPRETATION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planet; Physics; Astrophysics; Giant planet; Flux (metallurgy); Astronomy; Infrared; Planetary system; Super-Earth","score_opus":0.011304278484208561,"score_gpt":0.24373325770150375,"score_spread":0.2324289792172952,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099526242","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99082786,0.0014216489,0.0034105452,0.00040695976,0.00002517246,0.000010268013,0.00013121053,0.00017936285,0.0035870997],"genre_scores_gemma":[0.99667066,0.00023811149,0.0026888887,0.00007441184,0.000024324412,0.0000044295844,0.00009246785,0.000009664073,0.00019700661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998739,0.0000134757465,0.000008901405,0.000045531553,0.000021860513,0.000036354097],"domain_scores_gemma":[0.9992792,0.00024438958,0.00021601579,0.00009902287,0.000064080225,0.00009739511],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024977585,0.00030992128,0.00022026502,0.0010427912,0.0007290363,0.000708066,0.0006651633,0.00079100556,0.0020590217],"category_scores_gemma":[0.0009935768,0.0001767915,0.00019159674,0.00049331266,0.00077092217,0.00081002526,0.00055218645,0.0004209974,0.0003504912],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006010173,0.00009277775,0.6020491,0.0003384947,0.00008025402,0.0027364609,0.0009500392,0.00041090744,0.34356964,0.0015309477,0.0010234017,0.046616998],"study_design_scores_gemma":[0.000020342812,0.00010117934,0.94348496,0.000043043972,0.00006431074,0.0043523833,0.0008620124,0.0024226315,0.042174373,0.0018099081,0.0046434435,0.00002142025],"about_ca_topic_score_codex":0.0010698636,"about_ca_topic_score_gemma":0.0014829992,"teacher_disagreement_score":0.0020590217,"about_ca_system_score_codex":0.00038115543,"about_ca_system_score_gemma":0.00013429894,"threshold_uncertainty_score":0.0068880916},"labels":[],"label_agreement":null},{"id":"W2099613694","doi":"10.1086/375487","title":"The Sunyaev‐Zeldovich Effect Signature of Excess Entropy in Distant, Massive Clusters","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Intracluster medium; Astrophysics; Scaling; Galaxy cluster; Sunyaev–Zel'dovich effect; Entropy (arrow of time); Galaxy; Thermodynamics; Geometry","score_opus":0.0033501844405748452,"score_gpt":0.20652618049637872,"score_spread":0.2031759960558039,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099613694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991702,0.000060291834,0.000073227275,0.000010830822,0.000001024152,7.258628e-7,0.000035707933,0.000010502349,0.0006374965],"genre_scores_gemma":[0.9998599,0.000017624336,0.000031307747,0.0000028355237,0.0000035928601,5.13155e-7,0.000042698248,0.0000019490517,0.000039528008],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999242,0.000008876742,0.000004539369,0.000027128945,0.000016678006,0.000018605713],"domain_scores_gemma":[0.99923205,0.00015804588,0.00029066758,0.00010372308,0.000032492542,0.0001830157],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018451097,0.00015467603,0.00025283796,0.0010264843,0.000312256,0.00063931145,0.00022129041,0.0001240646,0.00083732774],"category_scores_gemma":[0.00089882786,0.00014905252,0.00010218569,0.0003699067,0.00085680233,0.00026263992,0.00069907133,0.00018601563,0.00010849279],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039701734,0.000028077333,0.9547265,0.000051056442,0.00006686927,0.00030895515,0.000851833,0.0014906017,0.028876701,0.004351107,0.00036894204,0.008482286],"study_design_scores_gemma":[0.0000063911843,0.000020964682,0.9973214,0.0000030362135,0.00001042209,0.00010810406,0.00007108696,0.00059192965,0.0008377253,0.00085116504,0.0001722763,0.000005470581],"about_ca_topic_score_codex":0.0015330535,"about_ca_topic_score_gemma":0.0013437171,"teacher_disagreement_score":0.0015330535,"about_ca_system_score_codex":0.0002315899,"about_ca_system_score_gemma":0.0001166087,"threshold_uncertainty_score":0.0030482411},"labels":[],"label_agreement":null},{"id":"W2099823767","doi":"10.1086/340063","title":"An Analytical Approach to Inhomogeneous Structure Formation","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Formalism (music); Structure formation; Halo; Galaxy; Dark matter; Redshift; Observable; Halo mass function; Cosmology; Nonlinear system","score_opus":0.011486436482421742,"score_gpt":0.21550045639025225,"score_spread":0.20401401990783052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2099823767","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.015330857,0.0002657307,0.9758577,0.00026971157,0.000031535044,0.000030100508,0.000083022234,0.00013138023,0.007999921],"genre_scores_gemma":[0.6600329,0.0019928995,0.31808963,0.0005398206,0.0004198654,0.00031794625,0.00024070073,0.00037088717,0.017995303],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99957687,0.00010684916,0.000017580021,0.00006837518,0.00015479664,0.000075430486],"domain_scores_gemma":[0.9983382,0.00062393094,0.00036689715,0.00027543397,0.00027688907,0.00011847917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010565465,0.0006412147,0.0006310813,0.0018751436,0.0006138415,0.0009902027,0.0023566375,0.00061479385,0.002525099],"category_scores_gemma":[0.005610537,0.00043563245,0.0009879486,0.001049758,0.0012813178,0.0022999463,0.0018850744,0.001035879,0.0006155678],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000058891615,0.00002655472,0.001345685,0.000040629282,0.000022540526,0.00016881518,0.00020822349,0.1836486,0.002396968,0.8027717,0.0009812972,0.00838312],"study_design_scores_gemma":[0.0000037038187,0.000012295139,0.00052093103,0.000011777988,0.000009657672,0.00011570307,0.000026361662,0.75250965,0.0005652138,0.24278648,0.0034203914,0.0000177843],"about_ca_topic_score_codex":0.0036097222,"about_ca_topic_score_gemma":0.002368641,"teacher_disagreement_score":0.0036097222,"about_ca_system_score_codex":0.0012945265,"about_ca_system_score_gemma":0.0010004153,"threshold_uncertainty_score":0.00939244},"labels":[],"label_agreement":null},{"id":"W2100107507","doi":"10.1086/508860","title":"Substructure around M31: Evolution and Effects","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Toronto","funders":"","keywords":"Surface brightness; Substructure; Population; Galaxy; Velocity dispersion; Dark matter; Halo; Dark matter halo; RADIUS; Satellite galaxy","score_opus":0.002718328648501702,"score_gpt":0.1825897200643555,"score_spread":0.17987139141585382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2100107507","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965155,0.00003802167,0.000079752455,0.0000120108625,4.8721665e-7,0.00000173291,0.000038241567,0.0000058570554,0.00017231621],"genre_scores_gemma":[0.99971646,0.000021645736,0.00007132668,0.000003041497,7.155123e-7,7.5423685e-7,0.00009478338,0.0000025525653,0.00008861643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999161,0.000022836355,0.0000036161384,0.000027454635,0.000010275399,0.000019853458],"domain_scores_gemma":[0.99924076,0.00020807776,0.00021854872,0.00007453808,0.00006446477,0.00019357726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003152523,0.00026935176,0.00023168552,0.0004883631,0.00041460452,0.00057436747,0.00040462922,0.000476048,0.00086451933],"category_scores_gemma":[0.0016572137,0.00015142624,0.00025345053,0.00045255004,0.00038757495,0.00029733955,0.0004664115,0.00020308046,0.00024427474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002684446,0.00009262937,0.92265534,0.000028184673,0.000096292664,0.0006349767,0.00025194813,0.054435983,0.014729569,0.0008254462,0.00022143038,0.0057596676],"study_design_scores_gemma":[0.000028958744,0.00030956182,0.87592834,0.0000102811055,0.00005158576,0.0005951627,0.0002787878,0.11887299,0.0025200413,0.00076558196,0.0006184624,0.00002031716],"about_ca_topic_score_codex":0.009330446,"about_ca_topic_score_gemma":0.006813418,"teacher_disagreement_score":0.009330446,"about_ca_system_score_codex":0.0005785622,"about_ca_system_score_gemma":0.00017208487,"threshold_uncertainty_score":0.018552303},"labels":[],"label_agreement":null},{"id":"W2100565482","doi":"10.1088/0004-637x/707/2/1595","title":"THE BIMODAL GALAXY STELLAR MASS FUNCTION IN THE COSMOS SURVEY TO<i>z</i>∼ 1: A STEEP FAINT END AND A NEW GALAXY DICHOTOMY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":149,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Lawrence Berkeley National Laboratory; Agence Nationale de la Recherche; Johns Hopkins University; California Institute of Technology","keywords":"Physics; Astrophysics; Stellar mass; Galaxy; Redshift; Astronomy; Star formation; Initial mass function; Supernova; Stars","score_opus":0.011588741846850527,"score_gpt":0.21788555442344884,"score_spread":0.20629681257659832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2100565482","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99847656,0.000107630935,0.00027194462,0.000038952614,0.0000017071256,0.0000012576037,0.00014477815,0.000017710201,0.0009394983],"genre_scores_gemma":[0.9995121,0.00004089185,0.00013575675,0.000015457515,0.000004920539,0.0000011161701,0.00020214297,0.0000043832893,0.000083240244],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999007,0.0000120419945,0.00000553811,0.0000339795,0.000017572975,0.00003026335],"domain_scores_gemma":[0.9994604,0.00007905144,0.00017316273,0.000054062133,0.000059179023,0.00017412053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003607152,0.00020449307,0.0002512081,0.0019091517,0.00020722313,0.00073329784,0.00019381414,0.00019482688,0.00091174676],"category_scores_gemma":[0.00068538554,0.00013166078,0.00019422147,0.0008060817,0.0005839351,0.00055411697,0.0006667738,0.0003548314,0.00024322451],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014619925,0.000013852042,0.9815824,0.000012450175,0.000020930505,0.00009427044,0.00040740197,0.0001897025,0.007580119,0.0007707805,0.00019085844,0.008991001],"study_design_scores_gemma":[0.0000017806855,0.000015462716,0.9988696,0.0000025176964,0.0000038852486,0.000060988597,0.000095857904,0.00023519357,0.0002437444,0.00019860988,0.00026965258,0.0000025945787],"about_ca_topic_score_codex":0.0030420173,"about_ca_topic_score_gemma":0.0044507645,"teacher_disagreement_score":0.0030420173,"about_ca_system_score_codex":0.00025473547,"about_ca_system_score_gemma":0.00012262675,"threshold_uncertainty_score":0.0060486197},"labels":[],"label_agreement":null},{"id":"W2100677756","doi":"10.1088/0004-637x/708/1/202","title":"THE COSMOS-WIRCam NEAR-INFRARED IMAGING SURVEY. I.<i>BzK</i>-SELECTED PASSIVE AND STAR-FORMING GALAXY CANDIDATES AT<i>z</i>≳ 1.4","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":250,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Galaxy; Redshift; Photometric redshift; Astronomy; Stars; Luminous infrared galaxy; Redshift survey","score_opus":0.004642214505805931,"score_gpt":0.20268154372452493,"score_spread":0.198039329218719,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2100677756","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.37650883,0.0014631104,0.003195503,0.0005345477,0.00013459312,0.00074020086,0.5531204,0.0014431179,0.06285971],"genre_scores_gemma":[0.22926538,0.001014867,0.0097066695,0.0002735925,0.000108644854,0.0006194511,0.7383221,0.00023365012,0.020455696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979013,0.000019036066,0.000014868602,0.000056555727,0.00008274467,0.00003664147],"domain_scores_gemma":[0.9992329,0.000028607481,0.00025145395,0.00009303716,0.00018666095,0.0002073705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041863942,0.00039964775,0.00034057544,0.0040215766,0.00028910572,0.00050187175,0.0005429436,0.00016664102,0.009568442],"category_scores_gemma":[0.00074516534,0.00023578777,0.0001736769,0.002828063,0.00015759155,0.00064631045,0.0009590024,0.00039237848,0.0065162387],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042342764,0.00021147287,0.638458,0.00039326842,0.00019055705,0.00018916215,0.00031640715,0.00028362824,0.0091593005,0.0028132834,0.26837096,0.07919058],"study_design_scores_gemma":[0.000038008282,0.000028475932,0.9153462,0.000033261716,0.000022058577,0.00013383204,0.00009555455,0.00029109506,0.0008926115,0.00020592751,0.082903445,0.000009435411],"about_ca_topic_score_codex":0.024611628,"about_ca_topic_score_gemma":0.043006018,"teacher_disagreement_score":0.024611628,"about_ca_system_score_codex":0.0005372101,"about_ca_system_score_gemma":0.00057361525,"threshold_uncertainty_score":0.048936725},"labels":[],"label_agreement":null},{"id":"W2100813785","doi":"10.1088/0004-637x/703/2/2108","title":"ROTATIONAL SPECTROSCOPY OF THE CO-PARA-H<sub>2</sub>MOLECULAR COMPLEX","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Rotational spectroscopy; Spectroscopy; van der Waals force; Microwave; Rotational transition; Molecular spectroscopy; Fourier transform spectroscopy; Atomic physics; Millimeter; Rotational–vibrational spectroscopy; Intermolecular force; Range (aeronautics); Astrophysics; Molecule; Astronomy; Excited state; Materials science","score_opus":0.007712645697120032,"score_gpt":0.2549322362589235,"score_spread":0.24721959056180345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2100813785","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970613,0.00013262496,0.0018016794,0.000036052388,0.0000044319463,0.000003917869,0.000044673863,0.000016509828,0.000898757],"genre_scores_gemma":[0.99862254,0.000068139496,0.0006785634,0.000012686024,0.0000036188662,0.000004134302,0.00006782111,0.000009428739,0.0005330477],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999044,0.000012781817,0.0000018281252,0.000025631512,0.000031445506,0.00002398381],"domain_scores_gemma":[0.99987245,0.000037700054,0.00004313849,0.000013931419,0.000017293889,0.000015480202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008103879,0.00015925351,0.000119610326,0.0001631584,0.00020928339,0.00019326531,0.0002216407,0.0002005193,0.00169682],"category_scores_gemma":[0.00028544254,0.00009713161,0.00006131231,0.00023190455,0.00030885148,0.00024217651,0.0001911249,0.00033049,0.00016738471],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011364591,0.000016019789,0.0012392801,0.000021962353,0.000007925751,0.00006800153,0.00006592543,0.000209354,0.9955214,0.00044017527,0.000059869828,0.002236241],"study_design_scores_gemma":[0.000029138248,0.00029799147,0.016784033,0.0000033576239,0.000017709244,0.00031176,0.00011021731,0.0038852275,0.97641754,0.00022592621,0.0019018645,0.000015398859],"about_ca_topic_score_codex":0.00047277962,"about_ca_topic_score_gemma":0.0004099579,"teacher_disagreement_score":0.00169682,"about_ca_system_score_codex":0.00016195945,"about_ca_system_score_gemma":0.000081590326,"threshold_uncertainty_score":0.0056764483},"labels":[],"label_agreement":null},{"id":"W2100858111","doi":"10.1086/423128","title":"A Search for TeV Gamma‐Ray Emission from High‐peaked Flat‐Spectrum Radio Quasars Using the Whipple Air Cerenkov Telescope","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Blazar; Physics; Astrophysics; Quasar; Telescope; Astronomy; Gamma ray; Galaxy","score_opus":0.014757084507608065,"score_gpt":0.2462806287773614,"score_spread":0.23152354426975333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2100858111","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9887079,0.0016174217,0.0036856416,0.00020113931,0.00002488769,0.00008482098,0.00063400576,0.00013740179,0.004906741],"genre_scores_gemma":[0.9902366,0.00080335274,0.0062388782,0.00023582965,0.00005269086,0.000024576613,0.001493275,0.000019359331,0.0008954431],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99952865,0.000047432182,0.000022328755,0.00013704383,0.00016802656,0.00009658371],"domain_scores_gemma":[0.9992318,0.00010439281,0.00030973664,0.00006836956,0.0000664821,0.00021921871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010335471,0.00040959657,0.00028438668,0.0022281883,0.0005847053,0.001120349,0.0005786857,0.00054254115,0.0012557942],"category_scores_gemma":[0.0008936295,0.00029331158,0.00042976526,0.0013680735,0.00033846617,0.0005337427,0.00073490577,0.0004638685,0.00036613463],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023316554,0.00017076562,0.8889114,0.00015349711,0.00022791135,0.0013977964,0.00070733624,0.00016522044,0.07246675,0.0007279294,0.00096767046,0.033870522],"study_design_scores_gemma":[0.000017930064,0.00016747226,0.993877,0.000027644797,0.000050833183,0.0011615326,0.00021595397,0.00027620196,0.0017034333,0.00018229427,0.0023081345,0.000011622007],"about_ca_topic_score_codex":0.0024255868,"about_ca_topic_score_gemma":0.003365336,"teacher_disagreement_score":0.0024255868,"about_ca_system_score_codex":0.00030140154,"about_ca_system_score_gemma":0.00034168994,"threshold_uncertainty_score":0.0054659843},"labels":[],"label_agreement":null},{"id":"W2100956118","doi":"10.1088/0004-637x/725/1/1165","title":"THE OPTICAL COMPANION TO THE BINARY MILLISECOND PULSAR J1824–2452H IN THE GLOBULAR CLUSTER M28","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; University of British Columbia","funders":"","keywords":"Globular cluster; Millisecond pulsar; Physics; Astrophysics; Pulsar; Pulsar planet; Binary pulsar; Astronomy; X-ray pulsar; Neutron star; Blue straggler; Stars","score_opus":0.008381925666434802,"score_gpt":0.23194498920376752,"score_spread":0.2235630635373327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2100956118","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99971086,0.000036614078,0.0000141251685,0.000005997663,9.846668e-7,7.5238705e-7,0.000014038402,0.0000013361962,0.00021529039],"genre_scores_gemma":[0.9995925,0.000037944006,0.0000655108,0.0000048546653,0.0000038939493,0.0000011968835,0.000076930715,7.9292414e-7,0.00021643494],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.0000053665794,0.0000036074553,0.000024665651,0.000022942771,0.000026462229],"domain_scores_gemma":[0.9998068,0.000016187463,0.000078103825,0.000027825467,0.00002305332,0.000048121445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000083076535,0.00015471055,0.00016148512,0.00069105165,0.00053951744,0.0003435968,0.0003240399,0.00022595903,0.00069316634],"category_scores_gemma":[0.00039747235,0.00010606009,0.00007197212,0.00041060874,0.0003578837,0.00017782023,0.000721864,0.00014413474,0.0002811347],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025486297,0.00008032126,0.9028336,0.000055167893,0.000036301957,0.005440407,0.0013276439,0.000261389,0.074421264,0.000257339,0.0004255791,0.014606137],"study_design_scores_gemma":[0.000011910323,0.00017603116,0.9851382,0.0000053887875,0.000019753104,0.0058725113,0.0007822268,0.0004020415,0.005125594,0.00016632363,0.0022921183,0.000007936044],"about_ca_topic_score_codex":0.0033450015,"about_ca_topic_score_gemma":0.0038674085,"teacher_disagreement_score":0.0033450015,"about_ca_system_score_codex":0.00024238347,"about_ca_system_score_gemma":0.00015064827,"threshold_uncertainty_score":0.0066511035},"labels":[],"label_agreement":null},{"id":"W2101000537","doi":"10.1088/0004-637x/784/2/87","title":"EVOLUTION OF ACCRETION DISKS IN TIDAL DISRUPTION EVENTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Accretion (finance); Light curve; Precession; Debris disk; Accretion disc; Black hole (networking); Intermediate polar; Supermassive black hole; Thick disk","score_opus":0.010155925710466137,"score_gpt":0.24220188541965595,"score_spread":0.23204595970918981,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101000537","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99805707,0.00015729739,0.0005915683,0.00003578488,0.000004420611,0.000008846953,0.00013124217,0.000019520916,0.0009942403],"genre_scores_gemma":[0.99930096,0.000044608714,0.00023490142,0.00000805787,0.0000027338322,0.0000036312915,0.00014385718,0.000007125064,0.00025417536],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989986,0.00001723509,0.000009184853,0.000032446267,0.00001642676,0.000024818433],"domain_scores_gemma":[0.9995552,0.00008462395,0.00014553455,0.000038197097,0.00006960996,0.00010694226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026291853,0.0002692511,0.00032616575,0.0008583287,0.00063863455,0.0012022079,0.0005136563,0.00060042937,0.00073134614],"category_scores_gemma":[0.0015599768,0.00028078674,0.00031073787,0.00041795394,0.0003898628,0.00051925634,0.0005988109,0.0002679438,0.00026382023],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006670384,0.00018593551,0.76430005,0.0000963783,0.00016087358,0.002489617,0.0006963229,0.138129,0.073606156,0.0051840195,0.0007401941,0.013744449],"study_design_scores_gemma":[0.00006735356,0.00021652089,0.5527419,0.000034189026,0.00007106407,0.0011506287,0.0006092729,0.42552826,0.011929042,0.0037821147,0.0037994224,0.00007019551],"about_ca_topic_score_codex":0.0047106678,"about_ca_topic_score_gemma":0.0020873502,"teacher_disagreement_score":0.0047106678,"about_ca_system_score_codex":0.0012769647,"about_ca_system_score_gemma":0.00020228367,"threshold_uncertainty_score":0.009366512},"labels":[],"label_agreement":null},{"id":"W2101053772","doi":"10.1088/0004-637x/785/1/43","title":"THE DISKMASS SURVEY. VIII. ON THE RELATIONSHIP BETWEEN DISK STABILITY AND STAR FORMATION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Star formation; Astrophysics; Stars; Scaling; Galaxy; Star (game theory); Stability (learning theory); Mathematics; Geometry","score_opus":0.04012169427060248,"score_gpt":0.26187570021553563,"score_spread":0.22175400594493316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101053772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.55046725,0.0030051593,0.0037232337,0.0008347175,0.00007969013,0.00010866691,0.42069927,0.00068172923,0.020400334],"genre_scores_gemma":[0.6407925,0.0018783252,0.0064622173,0.00028521122,0.000105374296,0.0001831114,0.33263662,0.00013153197,0.01752517],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978596,0.00003643027,0.000020049409,0.000064190295,0.000059612714,0.000033844368],"domain_scores_gemma":[0.99909997,0.000117120035,0.00025815124,0.00012495337,0.0002716262,0.00012826419],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005171189,0.00029389607,0.0002290081,0.002371808,0.00015907365,0.0004154722,0.00035131833,0.00025707358,0.0035572825],"category_scores_gemma":[0.0012435563,0.00012567117,0.00015774295,0.0022370014,0.000092391696,0.00029210353,0.00041818013,0.00014808253,0.003673643],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001390257,0.00003625989,0.92363507,0.00015615627,0.00007967023,0.0000632192,0.00009302312,0.0005107334,0.002211851,0.0008159243,0.031917088,0.040341955],"study_design_scores_gemma":[0.000010907062,0.00002275513,0.9644457,0.00002496499,0.00001824855,0.00009907358,0.000076809556,0.0008457641,0.0006937468,0.0002172278,0.0335405,0.0000043255486],"about_ca_topic_score_codex":0.019394489,"about_ca_topic_score_gemma":0.035411295,"teacher_disagreement_score":0.019394489,"about_ca_system_score_codex":0.00044406852,"about_ca_system_score_gemma":0.0003026795,"threshold_uncertainty_score":0.038563192},"labels":[],"label_agreement":null},{"id":"W2101173990","doi":"10.1086/425644","title":"A Search for Discrete X‐Ray Spectral Features in a Sample of Bright γ‐Ray Burst Afterglows","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Afterglow; Spectral line; Gamma-ray burst; Galaxy; Line (geometry); Line-of-sight; Emission spectrum; Monte Carlo method","score_opus":0.009781164995813298,"score_gpt":0.25346731776884274,"score_spread":0.24368615277302944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101173990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995067,0.000025717278,0.00025292134,0.000008079022,6.5276555e-7,0.0000049538767,0.0001121849,0.000008181025,0.00008070863],"genre_scores_gemma":[0.9985868,0.000030407255,0.0006763625,0.000008405595,0.000005449787,0.000008500809,0.0006171627,0.000006704407,0.000060223538],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997068,0.000055628465,0.000035981026,0.00010698328,0.000049851864,0.000044716722],"domain_scores_gemma":[0.9984457,0.00068912876,0.00038942776,0.00016163492,0.000064182,0.00025002533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057572237,0.00022052706,0.00030363386,0.0015555463,0.00038981525,0.000903644,0.0003366208,0.0003726645,0.0012000095],"category_scores_gemma":[0.0016495915,0.00017101671,0.00041048505,0.00075454696,0.00040345523,0.00029871418,0.0007193544,0.00026905685,0.00017915519],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003935471,0.00010286253,0.9682266,0.000027354443,0.0001041656,0.00029854034,0.00022344291,0.0025029064,0.018484594,0.00042348166,0.00017316939,0.009039303],"study_design_scores_gemma":[0.000024412839,0.00022725243,0.9909395,0.0000061397022,0.000052092193,0.00041333147,0.00016978319,0.0056052185,0.0020198673,0.00020451988,0.00032660807,0.000011349105],"about_ca_topic_score_codex":0.0010925344,"about_ca_topic_score_gemma":0.0013496064,"teacher_disagreement_score":0.0015555463,"about_ca_system_score_codex":0.00014639973,"about_ca_system_score_gemma":0.00019391543,"threshold_uncertainty_score":0.004014492},"labels":[],"label_agreement":null},{"id":"W2101201386","doi":"10.1088/0004-637x/789/2/155","title":"THE DISK AROUND THE BROWN DWARF KPNO TAU 3","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Accretion disc; Brown dwarf; Accretion (finance); Low Mass; High mass","score_opus":0.008583311245413438,"score_gpt":0.22938438378040213,"score_spread":0.22080107253498868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101201386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998243,0.00012643593,0.000121163146,0.00001623091,0.000002976876,0.0000033625724,0.00020603254,0.000027759195,0.001253099],"genre_scores_gemma":[0.9992494,0.00007201909,0.00020265144,0.000016328668,0.0000065324916,0.000001374973,0.00027500838,0.0000039183124,0.00017267355],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995923,0.000001195732,0.0000016021734,0.000014187521,0.000009659956,0.000014223882],"domain_scores_gemma":[0.99983466,0.000009790872,0.00008886183,0.000008614194,0.000015700163,0.00004229558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000051448445,0.00022119925,0.00016031941,0.0005379092,0.00048029263,0.00040867162,0.0002697205,0.00021211803,0.0006676004],"category_scores_gemma":[0.0001616862,0.00010627259,0.000115216484,0.00053931563,0.00018844477,0.00035183888,0.00031022134,0.0001548106,0.00027677047],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052690064,0.00008727592,0.8112003,0.00014872747,0.00007798781,0.0025990347,0.0015214022,0.0007641206,0.14857657,0.0007140111,0.0016456707,0.032137923],"study_design_scores_gemma":[0.000006334987,0.000055814093,0.99365884,0.000007671134,0.000016636232,0.00091100665,0.00021529756,0.0004249572,0.0023975258,0.00015687075,0.0021430515,0.000005930015],"about_ca_topic_score_codex":0.006200722,"about_ca_topic_score_gemma":0.0109894145,"teacher_disagreement_score":0.006200722,"about_ca_system_score_codex":0.0003970354,"about_ca_system_score_gemma":0.00013015985,"threshold_uncertainty_score":0.01232928},"labels":[],"label_agreement":null},{"id":"W2101439844","doi":"10.1088/0004-637x/795/1/27","title":"NON-ZEEMAN CIRCULAR POLARIZATION OF MOLECULAR MASER SPECTRAL LINES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Maser; Circular polarization; Spectral line; Polarization (electrochemistry); Antisymmetric relation; Scattering; Molecular cloud; Magnetic field","score_opus":0.005050623625086697,"score_gpt":0.21554262334126922,"score_spread":0.21049199971618252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101439844","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8016307,0.00024257317,0.18396999,0.00039094142,0.00004268803,0.000048374182,0.00012060163,0.0002744947,0.013279623],"genre_scores_gemma":[0.99464273,0.00014849727,0.0036706037,0.00001876357,0.000015958627,0.000010157929,0.000037183276,0.000015824668,0.0014401334],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999013,0.000020840034,0.000003159801,0.00002719396,0.000024368932,0.000023117853],"domain_scores_gemma":[0.99965346,0.00011306272,0.000084764986,0.000054814624,0.00005862161,0.00003526612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002661298,0.00035529464,0.00016994434,0.0004458136,0.00030941554,0.0003985606,0.00051071536,0.00034113647,0.0012982411],"category_scores_gemma":[0.0006774757,0.00017646627,0.00032659608,0.00027846178,0.0005679942,0.00063331705,0.00037616282,0.00027029045,0.00034505955],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039409156,0.0002297839,0.07156283,0.00020127652,0.00009372956,0.0026529622,0.00055467273,0.41505712,0.20741507,0.25852427,0.0015284058,0.041785847],"study_design_scores_gemma":[0.000013959196,0.000044597105,0.0066765896,0.0000035727785,0.000010060272,0.00046664328,0.000057877194,0.9595522,0.008727665,0.023860019,0.00056888594,0.000017797372],"about_ca_topic_score_codex":0.0014258539,"about_ca_topic_score_gemma":0.0010798213,"teacher_disagreement_score":0.0014258539,"about_ca_system_score_codex":0.00024350714,"about_ca_system_score_gemma":0.00026713416,"threshold_uncertainty_score":0.0043430924},"labels":[],"label_agreement":null},{"id":"W2101751945","doi":"10.1086/522880","title":"Seismology of Pre‐Main‐Sequence Stars in NGC 6530","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Stars; Astrophysics; Spectral line; Oscillation (cell signaling); Main sequence; Rotation (mathematics); Sequence (biology); Open cluster; Astronomy; Geometry","score_opus":0.014336949592536534,"score_gpt":0.2538138132053089,"score_spread":0.23947686361277234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101751945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997017,0.000027901324,0.00007273462,0.000004469413,6.781752e-7,0.0000013235243,0.00007424129,0.0000094354,0.00010745841],"genre_scores_gemma":[0.9996183,0.000015617907,0.00006389379,0.0000015056905,8.103704e-7,9.920499e-7,0.00026192327,0.000002382011,0.00003454301],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999126,0.000010950279,0.000010779668,0.00003083819,0.00001600255,0.00001891804],"domain_scores_gemma":[0.9996958,0.000045416076,0.000064788546,0.00003356074,0.00004004485,0.000120413584],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002918146,0.00035667096,0.00025072668,0.0008794227,0.00032588386,0.000378344,0.00035123446,0.0002939008,0.00047113397],"category_scores_gemma":[0.00071562105,0.00017324093,0.00035409018,0.0007026112,0.00023439804,0.00020760817,0.00046509155,0.00014792802,0.0001311423],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021230477,0.00006476962,0.93967515,0.000043627155,0.00008785479,0.00042269126,0.00055422797,0.03572633,0.016933834,0.00036813697,0.00025298522,0.0056580845],"study_design_scores_gemma":[0.000016857235,0.00008473712,0.9706261,0.0000056159743,0.000022656628,0.00012798865,0.00018217573,0.02804587,0.0005577757,0.00014524316,0.00017585153,0.000009156105],"about_ca_topic_score_codex":0.044183522,"about_ca_topic_score_gemma":0.05865946,"teacher_disagreement_score":0.044183522,"about_ca_system_score_codex":0.0007904649,"about_ca_system_score_gemma":0.00036646394,"threshold_uncertainty_score":0.08785272},"labels":[],"label_agreement":null},{"id":"W2101871480","doi":"10.1086/522826","title":"The Gemini Deep Planet Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":326,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto; Université de Montréal; National Research Council Canada; Université du Québec à Montréal","funders":"","keywords":"Physics; Planet; Stars; Astrophysics; Brown dwarf; Astronomy; Planetary system; Exoplanet; Planetary mass; Telescope","score_opus":0.013129219707182184,"score_gpt":0.23599709343366898,"score_spread":0.2228678737264868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101871480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6801531,0.0024861444,0.0050197844,0.0016920274,0.00015984685,0.0001958475,0.27829835,0.0018400971,0.030154943],"genre_scores_gemma":[0.6401358,0.0011001483,0.01299746,0.0006234209,0.00022814503,0.00019164142,0.32871056,0.00026715422,0.015745569],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958926,0.00008727339,0.000017190558,0.00012536939,0.0001021863,0.0000786448],"domain_scores_gemma":[0.9991874,0.00006928617,0.00017964508,0.00016480159,0.00015667995,0.00024223897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00082596124,0.00046770304,0.00026469905,0.0015292037,0.0003994767,0.00044776488,0.00037012206,0.00028168393,0.0036612377],"category_scores_gemma":[0.0009762187,0.00015420008,0.00018117695,0.0014569688,0.00011198064,0.00042176782,0.0010491817,0.00028584615,0.0024799742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010852232,0.0001645734,0.6521728,0.0002864895,0.0002324634,0.0003616538,0.00071128464,0.0017322568,0.011384029,0.0026350836,0.19877338,0.13046063],"study_design_scores_gemma":[0.00006661884,0.00012916679,0.7992967,0.000022604829,0.0000517257,0.0003854726,0.0001534628,0.0017280494,0.0018446287,0.0005925731,0.19571063,0.00001846614],"about_ca_topic_score_codex":0.0073764105,"about_ca_topic_score_gemma":0.009002458,"teacher_disagreement_score":0.0073764105,"about_ca_system_score_codex":0.0005395231,"about_ca_system_score_gemma":0.00040121705,"threshold_uncertainty_score":0.014666915},"labels":[],"label_agreement":null},{"id":"W2101873347","doi":"10.1086/318917","title":"Weak-Lensing Study of Low-Mass Galaxy Groups: Implications for Ω[TINF][ITAL]m[/ITAL][/TINF]","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Redshift; Weak gravitational lensing; Galaxy; Velocity dispersion; Cosmology; Mass ratio; Mass distribution; Luminosity; Universe; Galaxy group; RADIUS; Galaxy formation and evolution","score_opus":0.012249965002415951,"score_gpt":0.24355118469671294,"score_spread":0.23130121969429698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2101873347","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99546826,0.000091410635,0.00093162764,0.00005086526,0.0000021927538,0.000004156737,0.00012413056,0.0000205686,0.0033068715],"genre_scores_gemma":[0.99892175,0.000035366393,0.0005433526,0.0000067727815,0.0000050689423,0.000001327374,0.00021514508,0.000004416684,0.00026673725],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998293,0.000017858822,0.0000060913117,0.000033183413,0.00007374949,0.00003976442],"domain_scores_gemma":[0.998587,0.00020939593,0.0004759146,0.000115719944,0.00033895156,0.00027304547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005289478,0.00018267517,0.00019112744,0.0015697104,0.0005936697,0.00053983124,0.0006065371,0.00012105633,0.002741475],"category_scores_gemma":[0.0024567612,0.00007733024,0.00010073369,0.00078665634,0.0006114595,0.00031676923,0.000326588,0.00015479082,0.0004463247],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000829996,0.000041818847,0.9542926,0.000030136614,0.000042655403,0.00008611551,0.000349573,0.00096564257,0.011293787,0.0016505277,0.0003906212,0.030773474],"study_design_scores_gemma":[0.0000029039982,0.000039988303,0.99305576,0.0000037848374,0.000012095942,0.00007048167,0.00012529288,0.0032422342,0.0020392158,0.0005421948,0.000861748,0.0000043443397],"about_ca_topic_score_codex":0.05516894,"about_ca_topic_score_gemma":0.050290912,"teacher_disagreement_score":0.05516894,"about_ca_system_score_codex":0.0006548385,"about_ca_system_score_gemma":0.00037190857,"threshold_uncertainty_score":0.10969561},"labels":[],"label_agreement":null},{"id":"W2102069398","doi":"10.1088/0004-637x/707/2/1729","title":"BLAST: RESOLVING THE COSMIC SUBMILLIMETER BACKGROUND","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":176,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Redshift; Active galactic nucleus; Cosmic infrared background; Hubble Deep Field; Luminous infrared galaxy; Cosmic variance; Population; Telescope; Star formation; Infrared; Cosmic microwave background; Optics","score_opus":0.011044074729488481,"score_gpt":0.22173248217297759,"score_spread":0.2106884074434891,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102069398","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.064940035,0.0010135366,0.06009377,0.0023359489,0.00060127844,0.00035255146,0.6466731,0.14962643,0.07436341],"genre_scores_gemma":[0.21181804,0.00044495237,0.10466572,0.0009108045,0.0004434781,0.0004496571,0.6420763,0.025843019,0.013348011],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9993088,0.000109861176,0.000023858209,0.00011663263,0.00030749742,0.00013335956],"domain_scores_gemma":[0.9985349,0.0002919464,0.00011760644,0.00040218464,0.00028384986,0.00036945418],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017770233,0.001378257,0.0011834437,0.0026008997,0.0010977425,0.0016702191,0.0013737752,0.0010217752,0.051824097],"category_scores_gemma":[0.0021915263,0.0009571749,0.0009191626,0.0035053135,0.00033738496,0.0010290786,0.0017881979,0.0012447021,0.019225778],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015778303,0.0001833244,0.018059898,0.00029858382,0.00031548107,0.00042949,0.00029025323,0.007936429,0.023200171,0.006728774,0.8703099,0.070669875],"study_design_scores_gemma":[0.002191898,0.00034003847,0.11729023,0.00017999693,0.0004312927,0.000662625,0.00035652076,0.07318357,0.04996846,0.02803205,0.72703373,0.00032958886],"about_ca_topic_score_codex":0.00910444,"about_ca_topic_score_gemma":0.014020274,"teacher_disagreement_score":0.051824097,"about_ca_system_score_codex":0.0005150693,"about_ca_system_score_gemma":0.0008641647,"threshold_uncertainty_score":0.17336887},"labels":[],"label_agreement":null},{"id":"W2102326829","doi":"10.1088/0004-637x/705/2/l204","title":"PRE-DISCOVERY 2007 IMAGE OF THE HR 8799 PLANETARY SYSTEM","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Planet; Brown dwarf; Planetary system; Limit (mathematics); Flux (metallurgy); Debris; Debris disk; Field (mathematics)","score_opus":0.00571082916079724,"score_gpt":0.20558192770267078,"score_spread":0.19987109854187354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102326829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97375405,0.00025533905,0.001287577,0.00032554532,0.000035608024,0.00005399548,0.004773866,0.00028146637,0.019232415],"genre_scores_gemma":[0.9710515,0.00024901907,0.008883551,0.00021664677,0.00008182306,0.000035308345,0.012687128,0.000052055653,0.0067430036],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992645,0.0000034393402,0.0000035836508,0.000009455845,0.000029196526,0.000027853517],"domain_scores_gemma":[0.99980885,0.000015646276,0.000023873245,0.00003061532,0.000056279638,0.000064877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106026826,0.00011747073,0.00013742014,0.0011092536,0.00040441015,0.00035231785,0.00023307184,0.00042905918,0.00336157],"category_scores_gemma":[0.00014441884,0.00012266323,0.00015448913,0.00037487442,0.00009375707,0.00021012477,0.00037001673,0.00041141786,0.0011741923],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013303636,0.00077696913,0.30777004,0.00024285218,0.00012777153,0.004948921,0.0005852542,0.0016256698,0.55432963,0.001226612,0.04094805,0.086087905],"study_design_scores_gemma":[0.000016576529,0.00009081183,0.9760024,0.000014246331,0.000018919078,0.0014924135,0.000094530005,0.00078392983,0.011703419,0.00006493886,0.0097098015,0.0000081426915],"about_ca_topic_score_codex":0.0027778826,"about_ca_topic_score_gemma":0.011575579,"teacher_disagreement_score":0.00336157,"about_ca_system_score_codex":0.00025411716,"about_ca_system_score_gemma":0.00019567787,"threshold_uncertainty_score":0.011245608},"labels":[],"label_agreement":null},{"id":"W2102701958","doi":"10.1088/0004-637x/756/1/101","title":"SUBMILLIMETER OBSERVATIONS OF MILLIMETER BRIGHT GALAXIES DISCOVERED BY THE SOUTH POLE TELESCOPE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Redshift; Galaxy; Millimeter; South Pole Telescope; Astronomy; Spectral energy distribution; Source counts; Luminosity; Population; Line-of-sight; Submillimeter Array; Star formation","score_opus":0.01405047200748,"score_gpt":0.21147757083431093,"score_spread":0.19742709882683093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102701958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99155444,0.00026498066,0.0008505614,0.00006667972,0.00000837957,0.000019777748,0.002401174,0.00018082715,0.0046531777],"genre_scores_gemma":[0.9927101,0.00016562855,0.0023225837,0.0000616564,0.000036691577,0.000016102387,0.003930914,0.000023547174,0.00073277],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986625,0.0000096948,0.000004509619,0.000040702587,0.00004952694,0.000029240719],"domain_scores_gemma":[0.9993967,0.00006843957,0.00024884788,0.000093452974,0.000059631748,0.00013283205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019305608,0.00020013384,0.00024117668,0.0010816338,0.00036942674,0.00043126012,0.0004801107,0.00023540926,0.0014695312],"category_scores_gemma":[0.00047756132,0.00025714686,0.0002692819,0.000887517,0.00022359153,0.00019770821,0.00052230345,0.00033123,0.000603479],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033039818,0.00008990121,0.9103611,0.000093269904,0.00011885513,0.0007297776,0.0010256085,0.0008360027,0.051545035,0.00074491743,0.004914088,0.029211102],"study_design_scores_gemma":[0.000012507229,0.000039386327,0.99528474,0.0000048474312,0.000015679472,0.00025810595,0.00007012833,0.00044907135,0.0007001072,0.000060183113,0.0031007603,0.0000045584197],"about_ca_topic_score_codex":0.010016559,"about_ca_topic_score_gemma":0.028070794,"teacher_disagreement_score":0.010016559,"about_ca_system_score_codex":0.00045278284,"about_ca_system_score_gemma":0.0001757573,"threshold_uncertainty_score":0.019916534},"labels":[],"label_agreement":null},{"id":"W2102747712","doi":"10.1086/422336","title":"A Composite Extreme‐Ultraviolet QSO Spectrum from<i>FUSE</i>","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":207,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; QSOS; Physics; Redshift; Luminosity; Emission spectrum; Spectral line; Ultraviolet; Extreme ultraviolet; Astronomy; Galaxy; Optics","score_opus":0.008040965453859837,"score_gpt":0.19850732667804996,"score_spread":0.1904663612241901,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102747712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84559894,0.0005743243,0.0018391192,0.0027244845,0.0012477128,0.00019720287,0.030525034,0.002253047,0.11504011],"genre_scores_gemma":[0.9175432,0.0002533937,0.0030116322,0.0012972098,0.00068074284,0.00004689096,0.03672602,0.0005367226,0.03990417],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978,0.0000068175773,0.000009671636,0.000046940586,0.00009372619,0.00006294753],"domain_scores_gemma":[0.9987249,0.00012424779,0.0001770828,0.00012121944,0.00056194956,0.00029070073],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035954636,0.00028830997,0.00036235095,0.0016047308,0.0010175762,0.0006890548,0.00029800646,0.0008283305,0.022791823],"category_scores_gemma":[0.0007863198,0.00013386157,0.00028722463,0.0009967249,0.0001648751,0.0006091229,0.00045095908,0.00038308336,0.0044097616],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.006396144,0.0005936515,0.3338738,0.0007300722,0.0003190852,0.0074279546,0.0009963561,0.0010158926,0.2200637,0.0026551522,0.2984737,0.12745441],"study_design_scores_gemma":[0.000109895605,0.00026244935,0.9117934,0.00005175036,0.00010999584,0.0011589951,0.00036318297,0.0010403272,0.022596136,0.0005243016,0.06192826,0.00006134768],"about_ca_topic_score_codex":0.0033509426,"about_ca_topic_score_gemma":0.0075910585,"teacher_disagreement_score":0.022791823,"about_ca_system_score_codex":0.00028752684,"about_ca_system_score_gemma":0.0002016088,"threshold_uncertainty_score":0.07624626},"labels":[],"label_agreement":null},{"id":"W2102851019","doi":"10.1088/0004-637x/746/2/141","title":"VERITAS OBSERVATIONS OF DAY-SCALE FLARING OF M 87 IN 2010 APRIL","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Science Foundation; Science Foundation Ireland; U.S. Department of Energy; Office of Science; Smithsonian Institution","keywords":"Flare; Physics; Astrophysics; Flux (metallurgy); Spectral index; Galaxy; Spectral line; Astronomy","score_opus":0.01880063287137934,"score_gpt":0.22699186092565346,"score_spread":0.20819122805427412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102851019","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99104565,0.00017596688,0.00042080064,0.00008604171,0.000023582084,0.000021288713,0.0024993748,0.00016613056,0.0055610854],"genre_scores_gemma":[0.9869622,0.0001433647,0.0017630234,0.000103442195,0.00003474615,0.00001938721,0.008518268,0.000052536067,0.0024031417],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998124,0.000008133699,0.0000061093137,0.000034124838,0.00008510873,0.000054166394],"domain_scores_gemma":[0.99972934,0.000020074389,0.000067429675,0.000033448847,0.00009076632,0.000058864156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029483737,0.0002838295,0.00034259885,0.0010353872,0.0005278101,0.00046823433,0.00062832603,0.00041734247,0.00095833704],"category_scores_gemma":[0.00043063465,0.0002507898,0.00033609732,0.00072271,0.00020987811,0.0002198586,0.0007200584,0.00066156755,0.00038000822],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018092785,0.0003466122,0.6410622,0.00019765281,0.00035873032,0.0032075746,0.002220112,0.0035240834,0.28687024,0.0008517704,0.014158214,0.04539354],"study_design_scores_gemma":[0.000020541616,0.00009508308,0.99052167,0.0000141318,0.00003620944,0.00027911313,0.00012302623,0.0010613578,0.003358797,0.000034761357,0.0044425717,0.000012647974],"about_ca_topic_score_codex":0.030393021,"about_ca_topic_score_gemma":0.09441406,"teacher_disagreement_score":0.030393021,"about_ca_system_score_codex":0.0008946476,"about_ca_system_score_gemma":0.00038104027,"threshold_uncertainty_score":0.060432255},"labels":[],"label_agreement":null},{"id":"W2102937916","doi":"10.1088/0004-637x/753/1/23","title":"HerMES: A STATISTICAL MEASUREMENT OF THE REDSHIFT DISTRIBUTION OF HERSCHEL-SPIRE SOURCES USING THE CROSS-CORRELATION TECHNIQUE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Redshift; Luminous infrared galaxy; Redshift survey; Galaxy formation and evolution; Field galaxy; Hubble Deep Field; Sky; Photometric redshift","score_opus":0.01534165028463101,"score_gpt":0.2490621951578313,"score_spread":0.2337205448732003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2102937916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7030928,0.00055607886,0.19313751,0.00028206396,0.0000989183,0.00032244495,0.07325411,0.0106224185,0.018633708],"genre_scores_gemma":[0.8713503,0.00027713217,0.06457107,0.00014490896,0.0001530602,0.00026912856,0.058061153,0.0007642464,0.0044090254],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99851507,0.00031713737,0.00006294227,0.00046208457,0.0005183775,0.00012432621],"domain_scores_gemma":[0.99594814,0.0009008531,0.0010598202,0.0013106574,0.000541106,0.00023936431],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026723135,0.00063415535,0.0004776922,0.004967932,0.0003400414,0.0007630265,0.00084739615,0.00038763075,0.00390823],"category_scores_gemma":[0.0057631587,0.00036676187,0.00066258153,0.0031411361,0.00041786913,0.00080782146,0.0013855874,0.0004407928,0.0019122381],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034288396,0.00020080572,0.7790879,0.00024037353,0.0015448928,0.00024751588,0.00040315697,0.03642878,0.016840136,0.019806867,0.034540612,0.11031609],"study_design_scores_gemma":[0.000067985864,0.00011632479,0.8440299,0.000044480297,0.00013551752,0.0004340653,0.00012015339,0.104746975,0.014573635,0.006916049,0.028699078,0.00011588124],"about_ca_topic_score_codex":0.0074282675,"about_ca_topic_score_gemma":0.008439759,"teacher_disagreement_score":0.0074282675,"about_ca_system_score_codex":0.0005074866,"about_ca_system_score_gemma":0.00053362263,"threshold_uncertainty_score":0.014770031},"labels":[],"label_agreement":null},{"id":"W2103216761","doi":"10.1088/0004-637x/787/1/82","title":"A COMPREHENSIVE STUDY OF RELATIVISTIC GRAVITY USING PSR B1534+12","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":164,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Physics; Binary pulsar; Astrophysics; Precession; Neutron star; General relativity; Orbit (dynamics); Theory of relativity; Relativistic quantum chemistry; Jitter; Tests of general relativity; Gravitational-wave astronomy; Astronomy; Gravitational wave; Millisecond pulsar; Classical mechanics; Gravitational redshift; Quantum mechanics","score_opus":0.030596506040464082,"score_gpt":0.3444228419739501,"score_spread":0.313826335933486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103216761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99451447,0.0006049291,0.0022243222,0.000020524643,0.0000053795084,0.0000143096395,0.00064159586,0.00010546111,0.0018689953],"genre_scores_gemma":[0.98690414,0.0007777895,0.007446463,0.00003646426,0.000038633672,0.0000185049,0.0039882893,0.000057261055,0.00073259696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982125,0.00003370416,0.000014087606,0.00005555038,0.00004860291,0.000026850268],"domain_scores_gemma":[0.9995857,0.00006309419,0.00016113662,0.000079254154,0.00006535273,0.000045600114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056036434,0.0005026988,0.00040080014,0.0018351419,0.00037893417,0.00036093174,0.00042197778,0.00014813409,0.0004950598],"category_scores_gemma":[0.000757587,0.00017828541,0.00043662486,0.0025802169,0.00020321508,0.00022734662,0.0005511469,0.0001645028,0.00023365613],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059648784,0.00015594238,0.6867735,0.0004222456,0.0006115869,0.0015809245,0.0015722564,0.0058958097,0.16812332,0.0016725893,0.0015049155,0.13109045],"study_design_scores_gemma":[0.000011830233,0.00025209817,0.9857115,0.00001318222,0.00016003932,0.00082057854,0.0001246598,0.001828613,0.004985367,0.00022454816,0.0058383453,0.00002916337],"about_ca_topic_score_codex":0.010003021,"about_ca_topic_score_gemma":0.010083493,"teacher_disagreement_score":0.010003021,"about_ca_system_score_codex":0.00032232032,"about_ca_system_score_gemma":0.0003294902,"threshold_uncertainty_score":0.019889593},"labels":[],"label_agreement":null},{"id":"W2103263072","doi":"10.1086/375528","title":"The Broadband Optical Properties of Galaxies with Redshifts 0.02 &lt; <i>z</i> &lt; 0.22","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":761,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Astrophysics; Physics; Absolute magnitude; Surface brightness fluctuation; Magnitude (astronomy); Photometry (optics); Galaxy; Luminous infrared galaxy; Surface brightness; Brightest cluster galaxy; Fundamental plane (elliptical galaxies); Redshift; Elliptical galaxy; Brightness; Lenticular galaxy; Astronomy","score_opus":0.0074115569789030954,"score_gpt":0.18777391174913444,"score_spread":0.18036235477023135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103263072","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99117637,0.0002545552,0.0014182089,0.000029270457,0.0000034717339,0.000011350607,0.0031880867,0.00018501174,0.0037337882],"genre_scores_gemma":[0.9953458,0.00010864188,0.00049431674,0.00001591801,0.000012902237,0.000010837267,0.0035099222,0.000015408827,0.0004862643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982786,0.000017964634,0.000013043538,0.000047509908,0.000044315322,0.000049305763],"domain_scores_gemma":[0.9977743,0.00038089755,0.001191827,0.00016932064,0.00021834498,0.0002652856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036918363,0.00038611918,0.00020971066,0.0034380616,0.00018994782,0.00064081326,0.00026276516,0.00028022888,0.0029096499],"category_scores_gemma":[0.0019403998,0.00019464715,0.00027282906,0.002428955,0.00043712748,0.00054977625,0.000512141,0.00026037727,0.00113909],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007172198,0.00003857722,0.9810463,0.00003567493,0.00006633825,0.000085030486,0.00020688053,0.0008396996,0.006384986,0.000550238,0.00080477505,0.009869864],"study_design_scores_gemma":[0.0000015325775,0.000017040742,0.998757,0.000001645334,0.0000080842265,0.00010247229,0.000027010714,0.0004125758,0.0002002739,0.00009806186,0.00037170708,0.0000025707757],"about_ca_topic_score_codex":0.0040286267,"about_ca_topic_score_gemma":0.005813383,"teacher_disagreement_score":0.0040286267,"about_ca_system_score_codex":0.00032945976,"about_ca_system_score_gemma":0.000097718104,"threshold_uncertainty_score":0.009733796},"labels":[],"label_agreement":null},{"id":"W2103355909","doi":"10.1088/0004-637x/796/2/120","title":"ALMA OBSERVATIONS OF A MISALIGNED BINARY PROTOPLANETARY DISK SYSTEM IN ORION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protoplanetary disk; Molecular cloud; Binary number; Line (geometry); Submillimeter Array; Orbital plane; Mass ratio; Turbulence; Plane (geometry); Binary star","score_opus":0.013780502884361081,"score_gpt":0.22495592810074605,"score_spread":0.21117542521638497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103355909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917954,0.000053583863,0.00013847408,0.000018521336,0.0000038101932,0.000004560844,0.00006327007,0.000020180407,0.0005180326],"genre_scores_gemma":[0.9990803,0.000019499714,0.00061786466,0.000014716909,0.000008282558,0.000004072607,0.00010604363,0.0000035938338,0.00014558811],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987006,0.000012469257,0.000006835366,0.00004547709,0.00003566499,0.000029524375],"domain_scores_gemma":[0.9997521,0.000028997376,0.0000709451,0.000029635867,0.00003414947,0.000084085324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016247701,0.00018319847,0.00026403888,0.0005835593,0.0005679893,0.00043572008,0.00038811457,0.0004141414,0.0005021665],"category_scores_gemma":[0.0005397947,0.00017772209,0.00012420393,0.0003673132,0.00023594158,0.0003539437,0.000686772,0.00025004963,0.00012396468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012651295,0.00025983294,0.61476254,0.00009152825,0.0001437975,0.0027792125,0.0015473332,0.0016992859,0.35154706,0.00051146164,0.00057743216,0.024815386],"study_design_scores_gemma":[0.000041123265,0.00021317293,0.98901397,0.000010184674,0.000045970344,0.0008032183,0.00029074802,0.0040020905,0.0037500248,0.0001893289,0.0016258565,0.000014246002],"about_ca_topic_score_codex":0.0036074694,"about_ca_topic_score_gemma":0.005959529,"teacher_disagreement_score":0.0036074694,"about_ca_system_score_codex":0.00035910838,"about_ca_system_score_gemma":0.00017512197,"threshold_uncertainty_score":0.007172942},"labels":[],"label_agreement":null},{"id":"W2103613230","doi":"10.1088/0004-637x/783/2/131","title":"PROPERTIES OF THE REMNANT CLOCKWISE DISK OF YOUNG STARS IN THE GALACTIC CENTER","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":179,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Stars; Thick disk; Galactic Center; Thin disk; Galaxy; Kinematics; Laser guide star; Eccentricity (behavior); Galactic plane","score_opus":0.011183746615827052,"score_gpt":0.21504720266371527,"score_spread":0.20386345604788822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103613230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984894,0.00008128931,0.0012305995,0.000005067976,5.3794474e-7,0.0000013662677,0.00005883624,0.00001826706,0.00011461914],"genre_scores_gemma":[0.99905235,0.000035969304,0.00068215973,0.0000019530087,0.0000015766658,0.0000013655592,0.0001801801,0.0000050679714,0.00003945256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999,0.00002188931,0.0000081708295,0.000034806115,0.000020002724,0.000015047344],"domain_scores_gemma":[0.9994449,0.00010327372,0.0002380844,0.000078653844,0.0000823838,0.000052767078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032655685,0.0002657687,0.00023905057,0.0005798162,0.00022596098,0.00046732245,0.00045961142,0.00020464207,0.0001944329],"category_scores_gemma":[0.00110353,0.00018458329,0.00024935993,0.00041118768,0.00023105285,0.00038028962,0.00020638785,0.00011739168,0.00010544506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018133731,0.00003570304,0.9113363,0.000020027379,0.00006261939,0.00012932972,0.00018417397,0.064042546,0.015524143,0.0005784982,0.00009738106,0.0078081065],"study_design_scores_gemma":[0.000015144009,0.00010887135,0.6959313,0.000007015041,0.000044866327,0.0003231557,0.00006986876,0.29722673,0.005396376,0.0003729016,0.00048134473,0.000022473107],"about_ca_topic_score_codex":0.008145855,"about_ca_topic_score_gemma":0.0050729876,"teacher_disagreement_score":0.008145855,"about_ca_system_score_codex":0.000505149,"about_ca_system_score_gemma":0.0001205965,"threshold_uncertainty_score":0.016196907},"labels":[],"label_agreement":null},{"id":"W2103664113","doi":"10.1088/0004-637x/698/1/l56","title":"ASTEROSEISMOLOGY OF HYBRID PULSATORS MADE POSSIBLE: SIMULTANEOUS <i>MOST</i> SPACE PHOTOMETRY AND GROUND-BASED SPECTROSCOPY OF γ PEG","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Saint Mary's University; St. Mary's University; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Fonds Québécois de la Recherche sur la Nature et les Technologies; Austrian Science Fund","keywords":"Asteroseismology; Photometry (optics); Physics; Astrophysics; Spectroscopy; PEG ratio; Stars; Astronomy","score_opus":0.005983469308252512,"score_gpt":0.22725025986968792,"score_spread":0.2212667905614354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103664113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984499,0.00006205093,0.0006335545,0.00001540937,0.0000015404075,0.0000031072543,0.00014335958,0.00001490764,0.0006762066],"genre_scores_gemma":[0.9982468,0.0000351627,0.0013086251,0.000007766115,0.0000027220167,0.0000022778813,0.0002985636,0.000005269214,0.000092817616],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993527,0.000008985059,0.0000056225563,0.000028240045,0.000011985765,0.0000098219925],"domain_scores_gemma":[0.9997155,0.000035368277,0.000098873184,0.0000742421,0.00003348994,0.000042428335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018226038,0.00021119413,0.00015183035,0.0005963726,0.00022927902,0.0005281176,0.00021286157,0.00020815166,0.00067986426],"category_scores_gemma":[0.0003992782,0.00013368591,0.00014900518,0.00049474236,0.0002761974,0.0003722929,0.0005863623,0.00022498154,0.00015303529],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039157324,0.000059615933,0.7630946,0.00006524821,0.00009002844,0.0006770734,0.0008250227,0.0011394786,0.19074494,0.000602975,0.00020342354,0.04210606],"study_design_scores_gemma":[0.000022696497,0.00013592935,0.9735729,0.00001490652,0.00006087038,0.0016831609,0.00028266798,0.0023998609,0.019451726,0.0006216386,0.001740611,0.0000129164955],"about_ca_topic_score_codex":0.0006808174,"about_ca_topic_score_gemma":0.0011577763,"teacher_disagreement_score":0.0006808174,"about_ca_system_score_codex":0.00011470498,"about_ca_system_score_gemma":0.0000752117,"threshold_uncertainty_score":0.0022743344},"labels":[],"label_agreement":null},{"id":"W2103705762","doi":"10.1086/591928","title":"Reliable Identification of Compton‐thick Quasars at<i>z</i>≈ 2:<i>Spitzer</i>Mid‐Infrared Spectroscopy of HDF‐oMD49","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Canadian Space Agency; National Aeronautics and Space Administration; California Institute of Technology; Ames Research Center","keywords":"Physics; Quasar; Astrophysics; Active galactic nucleus; Spectroscopy; Redshift; Galaxy; Compton scattering; Infrared; Astronomy; Photometry (optics); Luminous infrared galaxy; Spectral energy distribution; Photon; Stars; Optics","score_opus":0.009021536932293604,"score_gpt":0.2194425039581086,"score_spread":0.210420967025815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103705762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964324,0.0002646927,0.00044100182,0.000040971994,0.000007945564,0.000009216331,0.00031234324,0.000029540082,0.0024618534],"genre_scores_gemma":[0.9984952,0.000087160995,0.00055966096,0.00004746577,0.00001452715,0.0000063118923,0.0005200103,0.000005804848,0.00026381126],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999798,0.000010538595,0.000015653419,0.00006111268,0.00005086074,0.000063885476],"domain_scores_gemma":[0.99931335,0.00007164799,0.00033003525,0.00007540313,0.00007725239,0.00013246275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033926233,0.00023083706,0.00022689078,0.0013725712,0.00039716598,0.0008179589,0.0003433162,0.00040241674,0.0012074059],"category_scores_gemma":[0.0005827561,0.00014056722,0.00020397935,0.00056872494,0.00033490857,0.0003633541,0.000753041,0.00029754484,0.00042165027],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010952449,0.000043130527,0.95448655,0.000028884535,0.00002287597,0.0007348286,0.00027011265,0.00007708935,0.035470128,0.00033132534,0.0003840953,0.008041354],"study_design_scores_gemma":[0.0000034091393,0.000015899675,0.99731964,0.0000049159585,0.00000872361,0.000422828,0.00007082353,0.00006474066,0.0013418027,0.000051231862,0.00069294136,0.0000030319432],"about_ca_topic_score_codex":0.0012647858,"about_ca_topic_score_gemma":0.0022050343,"teacher_disagreement_score":0.0013725712,"about_ca_system_score_codex":0.00022189932,"about_ca_system_score_gemma":0.00010405029,"threshold_uncertainty_score":0.0040391684},"labels":[],"label_agreement":null},{"id":"W2103790112","doi":"10.1086/500005","title":"Gemini Deep Deep Survey. VI. Massive Hδ‐strong Galaxies at<i>z</i>≃ 1","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Redshift; Balmer series; Sky; Stellar mass; Equivalent width; Population; Galaxy formation and evolution; Astronomy; Spectral line; Emission spectrum","score_opus":0.007378335458933498,"score_gpt":0.20662518626113333,"score_spread":0.19924685080219984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103790112","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.38087243,0.0016163924,0.0020268727,0.0029507594,0.00047805146,0.00034152338,0.5517547,0.0027831907,0.057176057],"genre_scores_gemma":[0.5515253,0.000620689,0.005642441,0.0015910624,0.00051624584,0.00019821845,0.3879648,0.000566657,0.051374648],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9998217,0.000013078235,0.000008621759,0.000040100847,0.00004372431,0.00007276784],"domain_scores_gemma":[0.9988803,0.00004990965,0.00020299337,0.00020609195,0.00015532426,0.0005053591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006747086,0.00064231805,0.00045919212,0.0013046222,0.0005674463,0.0006544923,0.00057071645,0.0005511104,0.011260562],"category_scores_gemma":[0.00070316315,0.0004894242,0.0003090606,0.0010576063,0.0001602375,0.00042987592,0.00085551577,0.00038938408,0.010082621],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010008028,0.0002770291,0.44269106,0.00036292803,0.00015230288,0.0004326557,0.0003037258,0.00035559808,0.015994323,0.00080269424,0.47580954,0.061817348],"study_design_scores_gemma":[0.000101924845,0.00006752104,0.91058236,0.000019678058,0.000060113987,0.00017264725,0.00009307654,0.00023743366,0.0017946456,0.0003592236,0.086496934,0.000014533039],"about_ca_topic_score_codex":0.015360739,"about_ca_topic_score_gemma":0.035902105,"teacher_disagreement_score":0.015360739,"about_ca_system_score_codex":0.00038896318,"about_ca_system_score_gemma":0.00043605498,"threshold_uncertainty_score":0.037670374},"labels":[],"label_agreement":null},{"id":"W2103987722","doi":"10.1088/0004-637x/790/1/40","title":"HerMES: THE REST-FRAME UV EMISSION AND A LENSING MODEL FOR THE<i>z</i>= 6.34 LUMINOUS DUSTY STARBURST GALAXY HFLS3","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Astronomical Observatories, Chinese Academy of Sciences; National Research Foundation; Science and Technology Facilities Council; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Danmarks Grundforskningsfond; National Science Foundation; Imperial College London; California Institute of Technology; National Aeronautics and Space Administration; Space Telescope Science Institute; UK Space Agency","keywords":"Physics; Galaxy; Astrophysics; Luminosity; Astronomy; Photometric redshift; Gravitational lens; Magnification; Redshift; Optics","score_opus":0.011571739399278245,"score_gpt":0.22098122879497792,"score_spread":0.20940948939569967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2103987722","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7417917,0.001274865,0.17565693,0.0023679684,0.00012234613,0.00017385112,0.0025635534,0.00091624854,0.07513245],"genre_scores_gemma":[0.9669389,0.0005269508,0.009299811,0.00014719328,0.00016444668,0.00010548844,0.0008853379,0.00013610169,0.021795722],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998816,0.000028844435,0.0000048026723,0.000026905489,0.0000299372,0.000027920189],"domain_scores_gemma":[0.9997807,0.000039978502,0.00007475417,0.000017836948,0.000023383032,0.00006340058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004401615,0.0008458352,0.00047749095,0.00085322454,0.0005842647,0.0011440531,0.0012375,0.0007889411,0.007412564],"category_scores_gemma":[0.00062594475,0.00031903473,0.0010704201,0.00032877666,0.00066635164,0.0012776454,0.0008610143,0.0005525247,0.0014547533],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003937741,0.00014083067,0.022864677,0.000090295354,0.00012386317,0.0010465581,0.00042898898,0.6303957,0.0077490974,0.3090113,0.0074065207,0.020348381],"study_design_scores_gemma":[0.00009551384,0.0000828003,0.008351851,0.000018433446,0.000026013504,0.00025871678,0.00009322833,0.92494017,0.00044063508,0.060868274,0.0047785603,0.00004590205],"about_ca_topic_score_codex":0.020982139,"about_ca_topic_score_gemma":0.007742374,"teacher_disagreement_score":0.020982139,"about_ca_system_score_codex":0.0012300841,"about_ca_system_score_gemma":0.00039441374,"threshold_uncertainty_score":0.041720033},"labels":[],"label_agreement":null},{"id":"W2104051788","doi":"10.1086/507983","title":"Search for Diffuse Astrophysical Neutrino Flux Using Ultra–High‐Energy Upward‐going Muons in Super‐Kamiokande I","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF","funders":"","keywords":"Physics; Muon; Neutrino; Flux (metallurgy); Neutrino detector; Nuclear physics; Muon neutrino; Astrophysics; Super-Kamiokande; Particle physics; Solar neutrino; Neutrino oscillation","score_opus":0.012789534288825068,"score_gpt":0.2364391164004661,"score_spread":0.22364958211164104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104051788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99906653,0.00008097663,0.00039541625,0.000012956915,0.0000014114119,0.0000024754308,0.000059863112,0.000008293549,0.00037204786],"genre_scores_gemma":[0.9985405,0.000092261056,0.0008245638,0.0000150650685,0.0000059942877,0.0000041844883,0.0003724843,0.000004209584,0.00014078923],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998148,0.00003609528,0.000010018348,0.000057104684,0.000035251098,0.00004670876],"domain_scores_gemma":[0.99910563,0.00027793428,0.00028109434,0.00010879787,0.0000943183,0.00013220277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048566156,0.0004031019,0.00040491877,0.0009210724,0.00040144505,0.00064821105,0.0002958544,0.00034671623,0.0010077591],"category_scores_gemma":[0.0010079814,0.00033472377,0.0003754291,0.0006483992,0.0002953753,0.0004475703,0.0007505175,0.0004406401,0.00016169266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069283607,0.00009901763,0.88495475,0.000060591912,0.00023111577,0.0010473941,0.0003874047,0.0011546058,0.101222605,0.0006038531,0.00014978772,0.009396068],"study_design_scores_gemma":[0.000030840783,0.00025996251,0.9707619,0.000021007714,0.00017331529,0.0013311865,0.0003312645,0.0029603285,0.022178149,0.0005251142,0.0014022797,0.000024728597],"about_ca_topic_score_codex":0.0009600139,"about_ca_topic_score_gemma":0.0019061682,"teacher_disagreement_score":0.0010077591,"about_ca_system_score_codex":0.000153819,"about_ca_system_score_gemma":0.00015091122,"threshold_uncertainty_score":0.0033712983},"labels":[],"label_agreement":null},{"id":"W2104082832","doi":"10.1088/0004-637x/731/1/18","title":"RADIAL STELLAR PULSATION AND THREE-DIMENSIONAL CONVECTION. I. NUMERICAL METHODS AND ADIABATIC TEST CASES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Adiabatic process; Physics; Amplitude; Mechanics; Coordinate system; Convection; Classical mechanics; Kinetic energy; Constant (computer programming); Stellar pulsation; Stars; Astrophysics; Geometry; Mathematics; Optics; Computer science; Quantum mechanics","score_opus":0.02448528030976713,"score_gpt":0.2615319888680872,"score_spread":0.23704670855832008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104082832","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86048776,0.00059103966,0.115152895,0.0004823003,0.00007283208,0.00018631644,0.00039065987,0.00042053504,0.022215597],"genre_scores_gemma":[0.9702556,0.0001337736,0.028431337,0.000048530237,0.000016398688,0.00011163568,0.00008023489,0.00004731647,0.00087508396],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997813,0.00008570261,0.00001732303,0.000016121205,0.000063392814,0.00003615522],"domain_scores_gemma":[0.99926597,0.00037730997,0.00013049225,0.00009234244,0.00007956978,0.000054329914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047203907,0.00031305992,0.00034586366,0.00038906644,0.00064273144,0.0007073945,0.0008374929,0.00073433947,0.001294421],"category_scores_gemma":[0.0025623427,0.00023193726,0.00046767297,0.00044256425,0.0010655914,0.0004464492,0.0009428378,0.00043304905,0.00015238716],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014293606,0.000117777105,0.009235218,0.00011121769,0.0000337982,0.00039689205,0.00016112383,0.9198386,0.0058237268,0.054562073,0.00050850847,0.009068115],"study_design_scores_gemma":[0.000034089724,0.000027777487,0.0006660522,0.0000069884327,0.0000037937446,0.00005157453,0.000020140982,0.99313605,0.0016417815,0.003933698,0.0004705679,0.0000074417167],"about_ca_topic_score_codex":0.0041326964,"about_ca_topic_score_gemma":0.001527762,"teacher_disagreement_score":0.0041326964,"about_ca_system_score_codex":0.00054071436,"about_ca_system_score_gemma":0.0005705087,"threshold_uncertainty_score":0.008217275},"labels":[],"label_agreement":null},{"id":"W2104104231","doi":"10.1086/339316","title":"The Optical Luminosity Function of Virialized Systems","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Galaxy; Luminosity function; Luminosity; Mass-to-light ratio; Sky; Range (aeronautics); Universe; Galaxy formation and evolution; Astronomy","score_opus":0.010725240215238848,"score_gpt":0.20038535406672622,"score_spread":0.18966011385148737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104104231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957728,0.00012781523,0.0016518845,0.00001858689,0.0000010598417,0.0000034926627,0.00020452785,0.000037758156,0.002182023],"genre_scores_gemma":[0.9988966,0.00003260556,0.00046756674,0.000008440395,0.0000026616055,0.0000029744422,0.00030126542,0.000006158458,0.00028172033],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986947,0.000018662735,0.0000072782177,0.00003566402,0.000025943182,0.00004288417],"domain_scores_gemma":[0.9988519,0.00025038622,0.00037831266,0.0001443026,0.00018693744,0.00018818634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003472822,0.00018169993,0.00013618689,0.0014320184,0.00024539733,0.00077204546,0.00025531856,0.00013873399,0.0018222098],"category_scores_gemma":[0.0017217107,0.000108435794,0.00018033966,0.00059076137,0.00036405536,0.0005628193,0.00056971074,0.00014955264,0.0004313691],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023210666,0.000053097905,0.9195546,0.000048384703,0.000109727596,0.00011679005,0.0005776768,0.006025466,0.038416542,0.0052475515,0.0004048894,0.029213196],"study_design_scores_gemma":[0.000010219307,0.00010305456,0.9729508,0.000010195603,0.000038771417,0.0003351624,0.00014038442,0.013669222,0.008488862,0.0024035217,0.0018320384,0.000017669017],"about_ca_topic_score_codex":0.0020190272,"about_ca_topic_score_gemma":0.0012936101,"teacher_disagreement_score":0.0020190272,"about_ca_system_score_codex":0.00053174305,"about_ca_system_score_gemma":0.00013286153,"threshold_uncertainty_score":0.006095886},"labels":[],"label_agreement":null},{"id":"W2104197395","doi":"10.1088/0004-637x/734/1/17","title":"A STUDY OF THE PHOTOMETRIC VARIABILITY OF THE PECULIAR MAGNETIC WHITE DWARF WD 1953–011","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Balmer series; White dwarf; Magnetic flux; Observable; Flux (metallurgy); Spectral line; Starspot; Cataclysmic variable star","score_opus":0.01751960238083628,"score_gpt":0.2163853429613464,"score_spread":0.19886574058051013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104197395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991941,0.000081651204,0.00024459657,0.000008311156,0.0000029515572,0.0000034940308,0.00011845267,0.000012235766,0.0003342276],"genre_scores_gemma":[0.9988524,0.000050250546,0.0004612118,0.000006376053,0.000011456413,0.0000031477657,0.00049827195,0.000004000739,0.00011285173],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992347,0.000009009889,0.0000041652306,0.000032416225,0.000018839746,0.000012069655],"domain_scores_gemma":[0.99973327,0.000033312186,0.00010666967,0.000040475465,0.000026199476,0.00005999471],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001744638,0.00022729939,0.00023189659,0.0008735966,0.00033996912,0.0003583649,0.00022478278,0.000225626,0.00037830957],"category_scores_gemma":[0.00040734396,0.000103948936,0.00023867274,0.00075537426,0.00020344288,0.00018624014,0.00025068843,0.00016555566,0.00015231843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004881912,0.00025285053,0.7345023,0.00012910402,0.00023939798,0.0010521855,0.00078071374,0.0016583863,0.229388,0.0004903216,0.00045972058,0.030558785],"study_design_scores_gemma":[0.000008688563,0.00007299383,0.99483067,0.0000028141508,0.000030726114,0.0004204523,0.000059193382,0.0010873572,0.0027558082,0.000070599366,0.0006538618,0.0000069585435],"about_ca_topic_score_codex":0.0030060487,"about_ca_topic_score_gemma":0.0049968385,"teacher_disagreement_score":0.0030060487,"about_ca_system_score_codex":0.00033561143,"about_ca_system_score_gemma":0.00011718969,"threshold_uncertainty_score":0.005977094},"labels":[],"label_agreement":null},{"id":"W2104229058","doi":"10.1088/0004-637x/744/1/16","title":"THE RICH CIRCUMSTELLAR CHEMISTRY OF SMP LMC 11","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Asymptotic giant branch; Carbon star; Planetary nebula; Nebula; Astrophysics; Physics; Circumstellar envelope; Circumstellar disk; Torus; Stars; Carbon fibers; Circumstellar dust; Absorption (acoustics); Astrobiology; Chemistry; Astronomy; Materials science","score_opus":0.013495595311037218,"score_gpt":0.21634982439722247,"score_spread":0.20285422908618525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104229058","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99834347,0.000055192777,0.00006169031,0.000019210573,0.0000010662627,0.0000025110432,0.00016695904,0.000014150986,0.001335738],"genre_scores_gemma":[0.99908566,0.00008831912,0.00018791272,0.000018539018,0.000004081572,0.0000047024864,0.00033971318,0.0000044047547,0.00026665026],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999567,0.000003420345,0.000002204389,0.000016458742,0.00000995991,0.000011195729],"domain_scores_gemma":[0.999918,0.0000099966555,0.0000291955,0.0000065871145,0.000007991156,0.000028240715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006536078,0.0003076436,0.0002240839,0.00048021413,0.0005255272,0.000445357,0.0002301334,0.00029000323,0.0011404493],"category_scores_gemma":[0.00019098973,0.00018726726,0.0001020843,0.00037040812,0.0003041246,0.00024568362,0.0003246342,0.00020124618,0.00028244389],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030946787,0.00009883921,0.46016222,0.00018453186,0.00008497451,0.0043295054,0.0002914987,0.00874191,0.51178044,0.0011717825,0.0011533913,0.011691398],"study_design_scores_gemma":[0.000016527718,0.00011275455,0.97862303,0.000012721935,0.000030981726,0.000900701,0.00020372805,0.0061412747,0.01186872,0.00018551013,0.0018890101,0.000015111172],"about_ca_topic_score_codex":0.0040763724,"about_ca_topic_score_gemma":0.0045143375,"teacher_disagreement_score":0.0040763724,"about_ca_system_score_codex":0.00054164446,"about_ca_system_score_gemma":0.0002068086,"threshold_uncertainty_score":0.008105278},"labels":[],"label_agreement":null},{"id":"W2104249489","doi":"10.1088/0004-637x/711/1/424","title":"PERSISTENT MAGNETIC WREATHS IN A RAPIDLY ROTATING SUN","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":226,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Dynamo; Tachocline; Solar dynamo; Convection zone; Magnetohydrodynamics; Dynamo theory; Convection; Buoyancy; Magnetism","score_opus":0.005176616795204399,"score_gpt":0.21308543786470346,"score_spread":0.20790882106949907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104249489","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986443,0.000031826665,0.00030804495,0.000045471832,0.0000061405535,0.0000056873005,0.000027701266,0.00002829111,0.0009024579],"genre_scores_gemma":[0.99946433,0.00003157335,0.000293047,0.000014037577,0.000003891082,0.000005235803,0.00004680205,0.00001176787,0.0001293119],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999318,0.000014653681,0.0000033349938,0.000010966773,0.000012277002,0.00002695235],"domain_scores_gemma":[0.9997625,0.000061391824,0.000045879173,0.000023009887,0.00002225323,0.00008494637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020611745,0.00022963958,0.00037905702,0.00024601648,0.00049321697,0.0006367751,0.00032031993,0.0004619408,0.00068622245],"category_scores_gemma":[0.0009909063,0.00020105363,0.00037451345,0.00018509544,0.00063451263,0.000369717,0.0005734012,0.00047095612,0.000081129714],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000700353,0.0003608347,0.09265928,0.000095574935,0.00022978324,0.0017221848,0.0006502601,0.8503223,0.03832293,0.0070356363,0.0012447021,0.006656254],"study_design_scores_gemma":[0.00022094374,0.00046461186,0.061623856,0.00002016234,0.00004686736,0.0002108095,0.00043132238,0.92963296,0.0032906947,0.0030157657,0.0010052144,0.000036806963],"about_ca_topic_score_codex":0.0051031387,"about_ca_topic_score_gemma":0.0040252474,"teacher_disagreement_score":0.0051031387,"about_ca_system_score_codex":0.00049576035,"about_ca_system_score_gemma":0.00038749367,"threshold_uncertainty_score":0.010146856},"labels":[],"label_agreement":null},{"id":"W2104258231","doi":"10.1086/424482","title":"The Compact Group of Galaxies HCG 31 in an Early Phase of Merging","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Galaxy; Kinematics; Dwarf galaxy; Galaxy rotation curve; Local Group; Compact group; Rotation (mathematics); Amplitude; Galaxy group","score_opus":0.010985816042409127,"score_gpt":0.25014221458655267,"score_spread":0.23915639854414356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104258231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99948275,0.000036423113,0.0000596221,0.0000054650177,5.85292e-7,0.000003602245,0.000023632403,0.00000349494,0.00038441503],"genre_scores_gemma":[0.99945134,0.000015166308,0.00019423003,0.000005574671,0.0000016910502,0.0000024658711,0.0001432116,0.0000012765169,0.00018517852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998301,0.000018984289,0.000007817856,0.0000415872,0.00003571387,0.0000656474],"domain_scores_gemma":[0.99950075,0.000055220615,0.00013354555,0.0000705145,0.00005141378,0.00018849905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002542994,0.00017115293,0.00029056642,0.00065962126,0.00050714734,0.00049285346,0.0002456916,0.00019713801,0.00068605895],"category_scores_gemma":[0.00066169584,0.000093452254,0.000104954015,0.0006333149,0.00056655623,0.00025449903,0.0007654538,0.00020837446,0.00023304984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00088913797,0.0001370231,0.8971707,0.000037652077,0.000052932104,0.0024713755,0.0023136493,0.0008926902,0.071102954,0.0015628469,0.00031370073,0.023055308],"study_design_scores_gemma":[0.000017887836,0.000336715,0.99180675,0.0000061317164,0.00001743016,0.0018120351,0.0006614557,0.00037990764,0.0026057647,0.00047354974,0.0018724692,0.00000985835],"about_ca_topic_score_codex":0.0041221376,"about_ca_topic_score_gemma":0.0042111287,"teacher_disagreement_score":0.0041221376,"about_ca_system_score_codex":0.00029764246,"about_ca_system_score_gemma":0.00022960061,"threshold_uncertainty_score":0.008196294},"labels":[],"label_agreement":null},{"id":"W2104398872","doi":"10.1088/0004-637x/756/2/134","title":"A DETAILED GRAVITATIONAL LENS MODEL BASED ON SUBMILLIMETER ARRAY AND KECK ADAPTIVE OPTICS IMAGING OF A<i>HERSCHEL</i>-ATLAS SUBMILLIMETER GALAXY AT<i>z</i>= 4.243<sup>,</sup><sup>,</sup>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Ciencia, Tecnología e Innovación Productiva; Academia Sinica; National Aeronautics and Space Administration; California Institute of Technology; Smithsonian Astrophysical Observatory; W. M. Keck Foundation; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Gravitational lens; Einstein radius; Submillimeter Array; Redshift; Einstein ring; Astronomy; Star formation","score_opus":0.012448792287896535,"score_gpt":0.2126052670250066,"score_spread":0.20015647473711007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104398872","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5684196,0.0011640448,0.3826823,0.001234519,0.00011203474,0.00020397762,0.0021473551,0.0008654274,0.0431708],"genre_scores_gemma":[0.9598644,0.00048841594,0.024383757,0.00014340285,0.00005679983,0.00011484028,0.0008903173,0.000102001955,0.013956163],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999856,0.000028325085,0.000006757776,0.00004501454,0.000038110113,0.000025662262],"domain_scores_gemma":[0.9998487,0.00002313159,0.00005248215,0.000015486039,0.000030615927,0.000029505562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018493191,0.0008084371,0.0004218127,0.00051623245,0.0004039867,0.00076048146,0.0013384612,0.0010453062,0.0023926026],"category_scores_gemma":[0.00046591825,0.0004326397,0.0007201161,0.00036328533,0.00039733734,0.001162065,0.0004388217,0.00041977633,0.0008955273],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000118331955,0.00005292314,0.01375584,0.00006104745,0.00012308273,0.00025522604,0.00015968867,0.9214386,0.011826032,0.04311262,0.0014919546,0.007604652],"study_design_scores_gemma":[0.000017557497,0.000030415807,0.0044147163,0.0000047432213,0.000024361552,0.000077751,0.000021849135,0.98947656,0.00050239114,0.004198714,0.001213932,0.000017109314],"about_ca_topic_score_codex":0.031624258,"about_ca_topic_score_gemma":0.019373095,"teacher_disagreement_score":0.031624258,"about_ca_system_score_codex":0.0014626837,"about_ca_system_score_gemma":0.0007598816,"threshold_uncertainty_score":0.0628804},"labels":[],"label_agreement":null},{"id":"W2104422604","doi":"10.1086/342242","title":"New CrH Opacities for the Study of L and Brown Dwarf Atmospheres","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Brown dwarf; Opacity; Molecular cloud; Line (geometry); Spectral line; Order (exchange)","score_opus":0.022103079033323533,"score_gpt":0.2335690890088149,"score_spread":0.21146600997549136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104422604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5144957,0.001119056,0.45916855,0.00027472558,0.00012994702,0.00009681381,0.0018203671,0.005040704,0.01785414],"genre_scores_gemma":[0.87310255,0.0004608512,0.12256344,0.00006984952,0.000095800766,0.000056228688,0.0010995765,0.00081973575,0.0017319797],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998661,0.000016843187,0.0000065315385,0.0000298099,0.00006399794,0.000016583353],"domain_scores_gemma":[0.99934095,0.00022291385,0.0001133443,0.00014287795,0.000115533745,0.00006442072],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037187757,0.00033995812,0.00023376329,0.0011436604,0.00037267394,0.0005490098,0.0006813198,0.0002959221,0.0020651703],"category_scores_gemma":[0.002116807,0.00020389847,0.00045009263,0.00060689135,0.00024607702,0.0011845665,0.00074052013,0.00060998445,0.0007149207],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015922484,0.00018586888,0.24254538,0.00040977838,0.00022391474,0.00040355042,0.00083115045,0.43365207,0.041006427,0.058529694,0.004366416,0.2176865],"study_design_scores_gemma":[0.000055344688,0.000059970986,0.059387695,0.000038593214,0.00005035415,0.00026711167,0.000115675626,0.88246125,0.017232861,0.013397574,0.026875943,0.000057510748],"about_ca_topic_score_codex":0.0044378126,"about_ca_topic_score_gemma":0.0051459884,"teacher_disagreement_score":0.0044378126,"about_ca_system_score_codex":0.00059668184,"about_ca_system_score_gemma":0.0004723386,"threshold_uncertainty_score":0.008823931},"labels":[],"label_agreement":null},{"id":"W2104508231","doi":"10.1086/528368","title":"X‐Ray and Near‐IR Variability of the Anomalous X‐Ray Pulsar 1E 1048.1−5937: From Quiescence Back to Activity","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Research Canada; Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Physics; Astrophysics; Pulsar; Flux (metallurgy); Magnetar; Black-body radiation; Glitch; Observatory; X-ray pulsar; Neutron star; Astronomy; X-ray; Telescope; Light curve; Radiation","score_opus":0.012970628898899324,"score_gpt":0.27942806519717367,"score_spread":0.26645743629827434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104508231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99720216,0.00040158833,0.000080397476,0.000027167822,0.000013377095,0.000005787834,0.0005958024,0.000020874919,0.0016528948],"genre_scores_gemma":[0.9954028,0.00043526688,0.00055098714,0.000048539998,0.000057234476,0.0000089686155,0.002371715,0.000019073039,0.0011053849],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999461,0.0000016472379,0.000004606823,0.00002009397,0.000015290887,0.000012217342],"domain_scores_gemma":[0.9998857,0.000009412706,0.000047550282,0.000012597971,0.000021050862,0.000023583654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008845614,0.00023564033,0.00022125746,0.00085372425,0.00028842324,0.0005135285,0.00021250852,0.00020354262,0.0011711312],"category_scores_gemma":[0.00022699272,0.00006238221,0.00011064357,0.0005452257,0.00022540495,0.00024086024,0.0004322811,0.00028862958,0.000402467],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036209723,0.00019426286,0.8291356,0.00014268758,0.00006375963,0.0019539972,0.00071588333,0.00037916482,0.10734595,0.0005976294,0.0028398433,0.05626901],"study_design_scores_gemma":[0.0000035540952,0.000058283713,0.99497163,0.000011832035,0.000011400579,0.000662177,0.00005490176,0.00011464006,0.0010104872,0.000062306135,0.003033745,0.000004912656],"about_ca_topic_score_codex":0.003031277,"about_ca_topic_score_gemma":0.004819138,"teacher_disagreement_score":0.003031277,"about_ca_system_score_codex":0.00027086912,"about_ca_system_score_gemma":0.00009901535,"threshold_uncertainty_score":0.0060272813},"labels":[],"label_agreement":null},{"id":"W2104659725","doi":"10.1088/0004-637x/730/1/22","title":"RADIO GALAXY NGC 1265 UNVEILS THE ACCRETION SHOCK ONTO THE PERSEUS GALAXY CLUSTER","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Radio galaxy; RADIUS; Shock wave; Population; Accretion (finance); Vorticity; Bow shock (aerodynamics); Galaxy","score_opus":0.012798169522156143,"score_gpt":0.20938544679514118,"score_spread":0.19658727727298503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104659725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9730645,0.00018153404,0.007148447,0.00027764894,0.000024646151,0.000019006042,0.00020402168,0.00015765693,0.018922618],"genre_scores_gemma":[0.9967332,0.00006560304,0.0011234109,0.00003549869,0.000012378124,0.0000063796833,0.000071284805,0.000011666961,0.0019405949],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999604,0.000007652128,0.0000016399352,0.000009663975,0.000009303527,0.000011271512],"domain_scores_gemma":[0.9999403,0.0000051685415,0.000018225377,0.000007756747,0.000005925248,0.000022626797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059683363,0.0004434792,0.00021253971,0.00021284392,0.0004523907,0.000805634,0.00067520613,0.00044298,0.0017622849],"category_scores_gemma":[0.00018255066,0.00015697292,0.0004449079,0.00017447295,0.00064097886,0.00040040622,0.0006054146,0.00025656942,0.00031001968],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003161205,0.000070407725,0.059932772,0.00007164517,0.000071820774,0.001999678,0.0007397592,0.8317441,0.011397,0.08273924,0.001980804,0.008936701],"study_design_scores_gemma":[0.0001342464,0.00017557321,0.04043041,0.000030169325,0.00006836955,0.000513208,0.00046623294,0.93532497,0.0012085506,0.017391454,0.004198504,0.000058320507],"about_ca_topic_score_codex":0.04527004,"about_ca_topic_score_gemma":0.015604538,"teacher_disagreement_score":0.04527004,"about_ca_system_score_codex":0.0013097129,"about_ca_system_score_gemma":0.00058075663,"threshold_uncertainty_score":0.09001303},"labels":[],"label_agreement":null},{"id":"W2104710165","doi":"10.1086/588542","title":"The Balloon‐borne Large Aperture Submillimeter Telescope (BLAST) 2005: Calibration and Targeted Sources","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Telescope; Calibration; Aperture (computer memory); Flux (metallurgy); Amplitude; Submillimeter Array; Submillimeter wave","score_opus":0.008305810040341014,"score_gpt":0.22502986102129033,"score_spread":0.21672405098094932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104710165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8436978,0.0027242647,0.0953993,0.00053124333,0.00019042597,0.00056893757,0.016853096,0.0036367357,0.03639829],"genre_scores_gemma":[0.84510076,0.0008304234,0.12260741,0.00027587276,0.00009097882,0.00039379578,0.02377831,0.0006029832,0.0063194386],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9993042,0.000071801245,0.0000371503,0.00017640757,0.000327943,0.00008254395],"domain_scores_gemma":[0.9991578,0.00005293506,0.00022461952,0.00019592952,0.00025304145,0.00011575871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019448957,0.00042692866,0.00045799342,0.0015456438,0.00090193993,0.0008145785,0.00078227196,0.0004962277,0.0020183567],"category_scores_gemma":[0.001298789,0.00041793103,0.00024899573,0.0023811676,0.0002579747,0.00038586784,0.0011778286,0.0007147378,0.0021753106],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017543188,0.0003101708,0.28705943,0.000505385,0.00015902158,0.0005989959,0.002055711,0.017711775,0.25786468,0.0060643796,0.033918954,0.3919972],"study_design_scores_gemma":[0.00013919584,0.00032780773,0.8756798,0.0001264249,0.000062859544,0.0010637473,0.00025332396,0.009529679,0.037466172,0.0012271783,0.07405114,0.000072654846],"about_ca_topic_score_codex":0.007593923,"about_ca_topic_score_gemma":0.011061426,"teacher_disagreement_score":0.007593923,"about_ca_system_score_codex":0.0015185399,"about_ca_system_score_gemma":0.00088647654,"threshold_uncertainty_score":0.015099466},"labels":[],"label_agreement":null},{"id":"W2104794972","doi":"10.1088/0004-637x/787/1/14","title":"DETECTING EXTRASOLAR MOONS AKIN TO SOLAR SYSTEM SATELLITES WITH AN ORBITAL SAMPLING EFFECT","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Exoplanet; Solar System; Transit (satellite); Planetary system; Stars; Celestial mechanics; Sampling (signal processing); Orbital inclination","score_opus":0.010087996305295959,"score_gpt":0.22715109014447857,"score_spread":0.2170630938391826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104794972","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9365567,0.00057746115,0.05834651,0.00007052355,0.000038967384,0.000027659777,0.00018475187,0.00036860962,0.003828922],"genre_scores_gemma":[0.984098,0.000109279514,0.014944676,0.000032794895,0.000022105962,0.000013498639,0.00017891126,0.000023888184,0.0005767849],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99973124,0.00005415745,0.000011366242,0.000091390044,0.00008805087,0.000023829358],"domain_scores_gemma":[0.9987851,0.0005402519,0.00028450481,0.00022718984,0.00011030224,0.000052668118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003924716,0.00018227291,0.0001710053,0.0005417854,0.00020104826,0.00031482702,0.00019813771,0.00026569905,0.0005431261],"category_scores_gemma":[0.0020334502,0.0001736991,0.00020251701,0.00045692964,0.00023803391,0.00029437055,0.0005633794,0.0001893984,0.00018128703],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006545614,0.00011444887,0.55914277,0.00017577743,0.0002604321,0.00040584157,0.00036041194,0.010262626,0.24119228,0.0027049077,0.00091172045,0.18381418],"study_design_scores_gemma":[0.000026187017,0.00050190394,0.7827319,0.000031105177,0.00015965413,0.0028786473,0.0001934086,0.0717535,0.1321846,0.0027280538,0.0067621185,0.00004898014],"about_ca_topic_score_codex":0.00041190244,"about_ca_topic_score_gemma":0.0013160193,"teacher_disagreement_score":0.0005431261,"about_ca_system_score_codex":0.00018109319,"about_ca_system_score_gemma":0.000099126075,"threshold_uncertainty_score":0.0020756125},"labels":[],"label_agreement":null},{"id":"W2104855000","doi":"10.1088/0004-637x/784/2/124","title":"THE DYNAMIC X-RAY NEBULA POWERED BY THE PULSAR B1259-63","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Pulsar; Nebula; Binary pulsar; Binary star; Outflow; Binary number; Circumbinary planet; Bow shock (aerodynamics); Pulsar wind nebula; Circular orbit","score_opus":0.005146685960976058,"score_gpt":0.21882621847340478,"score_spread":0.21367953251242872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104855000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99614465,0.00028827033,0.00017491651,0.000024801908,0.000007026188,0.000005500285,0.00015631967,0.000023314484,0.003175203],"genre_scores_gemma":[0.99931836,0.00007305292,0.00017316933,0.00001265057,0.000005235938,0.0000020190457,0.00020284991,0.0000037837256,0.00020892691],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999666,0.000002030756,0.0000015932746,0.000010136983,0.000010384245,0.000009312374],"domain_scores_gemma":[0.99993193,0.0000044799513,0.000022218997,0.0000069681737,0.0000045607185,0.000029913277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006427006,0.00016082237,0.00019609681,0.00051100994,0.00036409526,0.0004738098,0.000246788,0.00021137908,0.00070483604],"category_scores_gemma":[0.00015925913,0.00010511556,0.00010678488,0.00050445064,0.00023143053,0.00018901324,0.00052985817,0.00025031704,0.00021176902],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013996153,0.00035512605,0.38863835,0.00022910802,0.0001935174,0.0043843347,0.00059525727,0.003288977,0.54849607,0.003649237,0.0025836686,0.046186764],"study_design_scores_gemma":[0.00006587267,0.00013453887,0.98540556,0.0000197309,0.0000395358,0.0014314427,0.00010561678,0.0026382825,0.00566757,0.00058813835,0.0038871625,0.000016547481],"about_ca_topic_score_codex":0.0030717975,"about_ca_topic_score_gemma":0.005184991,"teacher_disagreement_score":0.0030717975,"about_ca_system_score_codex":0.00023633335,"about_ca_system_score_gemma":0.00009838945,"threshold_uncertainty_score":0.006107807},"labels":[],"label_agreement":null},{"id":"W2104885988","doi":"10.1088/0004-637x/779/1/18","title":"A SEARCH FOR FAST OPTICAL TRANSIENTS IN THE Pan-STARRS1 MEDIUM-DEEP SURVEY: M-DWARF FLARES, ASTEROIDS, LIMITS ON EXTRAGALACTIC RATES, AND IMPLICATIONS FOR LSST","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; National Aeronautics and Space Administration; Queen's University Belfast; Queen's University; Johns Hopkins University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Sky; Ecliptic; Light curve; Asteroid; Astronomy","score_opus":0.03236040124025293,"score_gpt":0.2853207834843646,"score_spread":0.2529603822441117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2104885988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987987,0.00010207832,0.00029876796,0.000027677477,0.0000011516225,0.0000068960617,0.00029938147,0.000018530602,0.00044672762],"genre_scores_gemma":[0.99831957,0.000058474474,0.0006278312,0.000012679104,0.000007100933,0.0000041836975,0.0008406788,0.0000043295386,0.00012518864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971443,0.00003688108,0.000020815009,0.00009230858,0.00007393537,0.000061629435],"domain_scores_gemma":[0.99858594,0.00027869854,0.0005792457,0.00014590933,0.00009649676,0.0003136422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074419205,0.00027183874,0.00029428385,0.00167053,0.0003452601,0.0007190586,0.00040853606,0.00041170363,0.0008792988],"category_scores_gemma":[0.0013556372,0.0001663164,0.00027803786,0.00081215263,0.00016779524,0.0003535392,0.0006701199,0.00023823827,0.00022757391],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103664235,0.000034530254,0.9817131,0.000025298048,0.00003822814,0.00019744941,0.00009296993,0.00035006806,0.00852001,0.00007503159,0.00012919113,0.008720518],"study_design_scores_gemma":[0.0000052946257,0.00006357706,0.9972095,0.0000055595415,0.000019995947,0.00028235203,0.0000917604,0.000978151,0.00086745777,0.000037033315,0.0004350701,0.0000042496113],"about_ca_topic_score_codex":0.0030407377,"about_ca_topic_score_gemma":0.0063052876,"teacher_disagreement_score":0.0030407377,"about_ca_system_score_codex":0.00027814205,"about_ca_system_score_gemma":0.00030956103,"threshold_uncertainty_score":0.0060460567},"labels":[],"label_agreement":null},{"id":"W2105041115","doi":"10.1086/426134","title":"Quasars and the Big Blue Bump","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Ultraviolet; Astrophysics; Quasar; Active galactic nucleus; Spectral index; Observatory; Spectral energy distribution; Astronomy; Spectral line; Extrapolation; Black hole (networking); Optics; Galaxy","score_opus":0.007094874080010401,"score_gpt":0.2054948790468317,"score_spread":0.1984000049668213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105041115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988696,0.00038040546,0.000111531335,0.00005522344,0.0000025533332,0.0000013256982,0.000046600024,0.000008514511,0.0005242368],"genre_scores_gemma":[0.9996345,0.00009019031,0.00006025896,0.000017561462,0.000012032831,8.775883e-7,0.00006369169,0.000002247839,0.000118654614],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99985385,0.000024628695,0.000005680672,0.000037646034,0.0000367407,0.000041365605],"domain_scores_gemma":[0.99851495,0.0002996663,0.0008291829,0.00008443179,0.00005461306,0.00021707868],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025572273,0.00028573224,0.00020463545,0.0010392823,0.00031581,0.00064857875,0.00024951095,0.00032073125,0.0020556932],"category_scores_gemma":[0.001006659,0.0001671713,0.00012710968,0.0005931708,0.000468525,0.0005660081,0.0005450368,0.00029890734,0.00023676615],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014815359,0.000043935135,0.9851151,0.000014780959,0.00003370706,0.0003931477,0.00038995914,0.00024065688,0.0023637437,0.00033593856,0.0002972705,0.010623496],"study_design_scores_gemma":[0.0000054912366,0.0000690197,0.99724114,0.0000064660385,0.000010362818,0.00066763116,0.0002458612,0.00056199037,0.0001841649,0.0005092243,0.0004941354,0.0000043770606],"about_ca_topic_score_codex":0.001248918,"about_ca_topic_score_gemma":0.0018694763,"teacher_disagreement_score":0.0020556932,"about_ca_system_score_codex":0.00017111523,"about_ca_system_score_gemma":0.000045546603,"threshold_uncertainty_score":0.006877005},"labels":[],"label_agreement":null},{"id":"W2105048043","doi":"10.1086/524647","title":"Comparative Analysis of Molecular Clouds in M31, M33, and the Milky Way","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Milky Way; Molecular cloud; Spiral galaxy; Galaxy; Andromeda; Local Group; Surface brightness","score_opus":0.013652695204121143,"score_gpt":0.25376991096102164,"score_spread":0.24011721575690048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105048043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997694,0.000032441134,0.000038814036,0.0000042213537,2.901295e-7,0.0000014543725,0.00003055201,0.0000034117234,0.00011948543],"genre_scores_gemma":[0.99953055,0.000029164099,0.00017582702,0.0000050546814,0.0000015730144,0.0000030584108,0.00020925405,0.0000020547736,0.000043502936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990416,0.000009065618,0.0000052139253,0.000025621193,0.000021633145,0.000034336445],"domain_scores_gemma":[0.9996929,0.00005675158,0.00010179283,0.000025980095,0.000027232305,0.00009536724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012930245,0.00013454992,0.0001841452,0.0008087095,0.00032661975,0.00039461683,0.00029974806,0.00023957352,0.000512398],"category_scores_gemma":[0.00042426313,0.00016630275,0.00025438744,0.0005577022,0.00018749255,0.00025436995,0.000386923,0.00013418245,0.00011124892],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005748224,0.0001296086,0.9347885,0.000038230366,0.00014418608,0.00041549458,0.0004318252,0.0085900845,0.04409471,0.0008809448,0.00024290722,0.0096687],"study_design_scores_gemma":[0.0000189294,0.000080938116,0.99120003,0.0000043071236,0.00002255971,0.00013071789,0.00011190453,0.006941995,0.0010773486,0.00008329984,0.00032234297,0.0000056665767],"about_ca_topic_score_codex":0.0076420717,"about_ca_topic_score_gemma":0.009907737,"teacher_disagreement_score":0.0076420717,"about_ca_system_score_codex":0.000511507,"about_ca_system_score_gemma":0.00020946805,"threshold_uncertainty_score":0.015195131},"labels":[],"label_agreement":null},{"id":"W2105139159","doi":"10.1088/0004-637x/730/2/68","title":"SPECTROSCOPY OF LUMINOUS<i>z</i>&gt; 7 GALAXY CANDIDATES AND SOURCES OF CONTAMINATION IN<i>z</i>&gt; 7 GALAXY SEARCHES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Physics; Redshift; Astrophysics; Galaxy; Photometry (optics); Population; Spectral energy distribution; Astronomy; Spectroscopy; Luminosity function; Stars","score_opus":0.010495761268461653,"score_gpt":0.21305731132295136,"score_spread":0.2025615500544897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105139159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998181,0.000107635715,0.0003299579,0.00003934491,0.0000027387541,0.0000108309805,0.00016738716,0.000031659176,0.0011294787],"genre_scores_gemma":[0.9969746,0.00011243159,0.001004411,0.000053376916,0.000009550078,0.000016509965,0.0013187035,0.000022125752,0.0004884032],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995646,0.000038875056,0.000031849948,0.00007382967,0.00014172735,0.00014920691],"domain_scores_gemma":[0.9980286,0.0001869828,0.00085916166,0.00021975215,0.0003140024,0.00039162507],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008098334,0.00034394782,0.0004981262,0.0020835635,0.00057080673,0.0011510953,0.000807798,0.00043940605,0.0013382119],"category_scores_gemma":[0.0014922986,0.00023150246,0.00032009557,0.0018239513,0.00042932242,0.0003905985,0.0009406449,0.00026319918,0.00065159483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027294498,0.000057075486,0.9714778,0.000054830885,0.000045645367,0.0005725367,0.00050140783,0.00024292489,0.015321987,0.0005110257,0.0006201524,0.010321551],"study_design_scores_gemma":[0.000014452752,0.00012788705,0.98990905,0.000027483953,0.00008413997,0.00082058617,0.00049234746,0.001100034,0.004894559,0.00023473939,0.0022840519,0.000010681435],"about_ca_topic_score_codex":0.003439357,"about_ca_topic_score_gemma":0.0061761816,"teacher_disagreement_score":0.003439357,"about_ca_system_score_codex":0.0006003881,"about_ca_system_score_gemma":0.00024884145,"threshold_uncertainty_score":0.0068386793},"labels":[],"label_agreement":null},{"id":"W2105266144","doi":"10.1086/499362","title":"<i>MOST</i> Detects <i>g</i> -Modes in the Be Star HD 163868","year":2005,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; St. Mary's University; University of Toronto; Université de Montréal; Saint Mary's University; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Stars; Opacity; Light curve; Star (game theory); Astronomy; Optics","score_opus":0.013739885444874098,"score_gpt":0.23010127754168194,"score_spread":0.21636139209680785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105266144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99769443,0.00005427992,0.0009537672,0.000024240548,0.0000029141731,0.000002663511,0.00030620856,0.00006925261,0.00089218403],"genre_scores_gemma":[0.9976972,0.00001669053,0.0015331415,0.000011769131,0.0000044862695,0.0000023712785,0.0005490134,0.000013416207,0.00017180952],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998975,0.000015312806,0.0000075851826,0.000035172343,0.000020916274,0.000023574396],"domain_scores_gemma":[0.9996846,0.000048727234,0.00010789226,0.000069472,0.000037565755,0.000051915296],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003103296,0.00016850646,0.00023095199,0.0007444836,0.00037048705,0.00039636355,0.00021556782,0.0002946825,0.0009557373],"category_scores_gemma":[0.00057106145,0.00016440054,0.00017229699,0.0003916938,0.00017220336,0.00017569061,0.0002488296,0.00018235044,0.00038623772],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003122935,0.000066584376,0.8119506,0.00006179031,0.00006073485,0.00033140738,0.00032272682,0.0027220834,0.15970199,0.0005770713,0.0007865998,0.023106098],"study_design_scores_gemma":[0.000008088347,0.000050383238,0.9822525,0.0000061298215,0.000022261263,0.00026804532,0.00004972337,0.00522071,0.010539471,0.00023558222,0.0013365964,0.000010427754],"about_ca_topic_score_codex":0.0016590569,"about_ca_topic_score_gemma":0.0033875145,"teacher_disagreement_score":0.0016590569,"about_ca_system_score_codex":0.00016495735,"about_ca_system_score_gemma":0.000070787755,"threshold_uncertainty_score":0.0032987595},"labels":[],"label_agreement":null},{"id":"W2105289892","doi":"10.1088/0004-637x/760/2/113","title":"A CLOSE-PAIR ANALYSIS OF DAMP MERGERS AT INTERMEDIATE REDSHIFTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Virial theorem; Halo; Redshift; Galaxy; Spectral line; Galaxy merger; Stars; Very Large Telescope","score_opus":0.007895155062786005,"score_gpt":0.22539775671638607,"score_spread":0.21750260165360005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105289892","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994574,0.00009025366,0.00013844062,0.000005968256,7.18404e-7,0.0000027512228,0.00008173763,0.000004280079,0.00021844314],"genre_scores_gemma":[0.99949,0.000021688704,0.00014108811,0.0000036056601,0.0000016306693,0.0000017502272,0.00020574254,0.000002058817,0.00013237704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996402,0.00007745762,0.00002206138,0.00010271708,0.00007065683,0.000086841115],"domain_scores_gemma":[0.9984315,0.00023364209,0.0005574305,0.00014438997,0.00018922087,0.00044380754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050539634,0.00018171934,0.00034059864,0.001958642,0.0006029354,0.0005768187,0.000316325,0.00021520021,0.0016018852],"category_scores_gemma":[0.0018462085,0.00015200187,0.00022274253,0.00094539067,0.0002475166,0.00044307398,0.0010292635,0.00021837861,0.0003942179],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019135671,0.000026346765,0.9884737,0.000011968156,0.000037911053,0.00023626965,0.00056861294,0.00013578686,0.0061123148,0.00022033005,0.0000820066,0.0039034702],"study_design_scores_gemma":[0.0000029521807,0.00006693307,0.9976787,0.0000028600696,0.000016934762,0.00030882464,0.00028827158,0.0005771315,0.0006603623,0.00005186353,0.00034093848,0.000004189022],"about_ca_topic_score_codex":0.003324598,"about_ca_topic_score_gemma":0.004273316,"teacher_disagreement_score":0.003324598,"about_ca_system_score_codex":0.00024782596,"about_ca_system_score_gemma":0.000111457564,"threshold_uncertainty_score":0.0066105127},"labels":[],"label_agreement":null},{"id":"W2105340146","doi":"10.1086/589618","title":"Three-dimensional Simulation of Magnetized Cloud Fragmentation Induced by Nonlinear Flows and Ambipolar Diffusion","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Physics; Turbulence; Magnetohydrodynamics; Magnetic field; Supersonic speed; Mechanics; Nonlinear system; Computational physics; Classical mechanics; Astrophysics; Plasma; Nuclear physics","score_opus":0.012289222202902461,"score_gpt":0.2407846838933158,"score_spread":0.22849546169041335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105340146","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9867077,0.0001010411,0.0045150276,0.000300809,0.00003757612,0.000047095924,0.0004239826,0.00013607451,0.007730636],"genre_scores_gemma":[0.9960408,0.00005759937,0.0027385347,0.00006358734,0.000011296757,0.000048309917,0.00022145595,0.0000306008,0.0007878804],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998685,0.000027039821,0.0000056814106,0.00001573964,0.000028137996,0.00005485079],"domain_scores_gemma":[0.99924797,0.00036942863,0.00010032936,0.000036491772,0.000082677645,0.00016314644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029251486,0.00042687,0.0005581378,0.00039289668,0.0007936312,0.000844407,0.0010319784,0.001034486,0.002032417],"category_scores_gemma":[0.0013200269,0.00032668735,0.00060682656,0.00043724876,0.00097612286,0.0004066731,0.00076325046,0.0008749248,0.00013740835],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014956061,0.00010591447,0.0041123703,0.000026107466,0.00004027877,0.00020418996,0.00008447621,0.99107003,0.0015166795,0.0017556933,0.0002220468,0.000712626],"study_design_scores_gemma":[0.000053766802,0.000025500009,0.0009951191,0.0000030293577,0.0000055324267,0.000010934582,0.000031340816,0.9981565,0.00023061859,0.00035310176,0.00012862975,0.0000058407545],"about_ca_topic_score_codex":0.03066417,"about_ca_topic_score_gemma":0.014711387,"teacher_disagreement_score":0.03066417,"about_ca_system_score_codex":0.0012065712,"about_ca_system_score_gemma":0.0010340534,"threshold_uncertainty_score":0.06097138},"labels":[],"label_agreement":null},{"id":"W2105535379","doi":"10.1086/422251","title":"The Identification of Blue Horizontal-Branch Stars in the Integrated Spectra of Globular Clusters","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Queen's University","funders":"","keywords":"Globular cluster; Horizontal branch; Balmer series; Astrophysics; Physics; Spectral line; Degeneracy (biology); Degenerate energy levels; Stars; Spectroscopy; Astronomy; Emission spectrum","score_opus":0.0071066079613074816,"score_gpt":0.21976192544782816,"score_spread":0.21265531748652067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105535379","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99737704,0.00022292136,0.0012561888,0.0000094697625,0.0000026054763,0.0000013227746,0.000063928244,0.000029984007,0.001036567],"genre_scores_gemma":[0.99851984,0.00006864767,0.0010882573,0.000007888962,0.0000033523097,0.0000014482542,0.00008361774,0.0000067482815,0.00022019837],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998969,0.000011096145,0.000005993621,0.000035468674,0.00003566384,0.000014924661],"domain_scores_gemma":[0.9994431,0.00012194375,0.00012387626,0.000081807266,0.00014722177,0.00008201185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002779586,0.00015599962,0.000123864,0.0009178695,0.00021866718,0.00065066986,0.00025906932,0.00024234902,0.0005933521],"category_scores_gemma":[0.0014062264,0.00012894906,0.00006256046,0.00071473606,0.0003225349,0.00046313394,0.0005428714,0.0001753218,0.0001699581],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000316674,0.000030550218,0.73808444,0.00008144402,0.00010758108,0.00023117161,0.00071477576,0.0016026439,0.21059936,0.0020698912,0.0002674822,0.045893975],"study_design_scores_gemma":[0.0000057010534,0.000042330023,0.97578025,0.000012476555,0.000038720456,0.00039646722,0.0002247405,0.0032295254,0.018480415,0.00091976614,0.0008613188,0.000008222954],"about_ca_topic_score_codex":0.0015010221,"about_ca_topic_score_gemma":0.0030558794,"teacher_disagreement_score":0.0015010221,"about_ca_system_score_codex":0.0002569724,"about_ca_system_score_gemma":0.00012096262,"threshold_uncertainty_score":0.0029845834},"labels":[],"label_agreement":null},{"id":"W2105640984","doi":"10.1086/427208","title":"Pulsar Birthrates from the Parkes Multibeam Survey","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"","keywords":"Pulsar; Physics; Astrophysics; Population; Luminosity; Astronomy; Millisecond pulsar; Galaxy; Demography","score_opus":0.018369053412647635,"score_gpt":0.3116395940540451,"score_spread":0.29327054064139746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105640984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971173,0.00016442442,0.00014947502,0.000015833417,0.0000017189692,0.0000059242284,0.002073102,0.000009110855,0.0004631978],"genre_scores_gemma":[0.9889591,0.00046581362,0.00031324613,0.000018363573,0.000009485032,0.000018504285,0.009431782,0.00001105639,0.0007726776],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999658,0.000055866687,0.00004343154,0.00008514137,0.000097467346,0.000060127368],"domain_scores_gemma":[0.9975128,0.0005666645,0.0011027462,0.0002675344,0.0003244402,0.00022579847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052934524,0.00018589383,0.00024510946,0.0023224861,0.00022668797,0.00041462312,0.00023635339,0.00018201118,0.0011777377],"category_scores_gemma":[0.002521465,0.00017498943,0.00022035767,0.0010932799,0.0001527717,0.0003800729,0.00072479196,0.00019522855,0.000501212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052072523,0.000006529722,0.9933351,0.000016075983,0.000031012303,0.000085374864,0.00017234735,0.00015048584,0.00076477113,0.000058752597,0.000241465,0.0050860345],"study_design_scores_gemma":[0.0000017798438,0.000016953654,0.9984327,0.0000031105244,0.0000068252143,0.00024741932,0.00005408004,0.00013311158,0.00022169622,0.000015647569,0.00086362154,0.0000030946264],"about_ca_topic_score_codex":0.0036553927,"about_ca_topic_score_gemma":0.005254917,"teacher_disagreement_score":0.0036553927,"about_ca_system_score_codex":0.00019314539,"about_ca_system_score_gemma":0.000105013576,"threshold_uncertainty_score":0.00726825},"labels":[],"label_agreement":null},{"id":"W2105731191","doi":"10.1088/0004-637x/782/1/13","title":"A THREE-YEAR MULTI-WAVELENGTH STUDY OF THE VERY-HIGH-ENERGY γ-RAY BLAZAR 1ES 0229+200","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Office of Science; California Institute of Technology; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution; Science Foundation Ireland; National Science Foundation","keywords":"Blazar; Physics; Crab Nebula; Intergalactic travel; Astrophysics; BL Lac object; Extragalactic background light; Active galactic nucleus; Fermi Gamma-ray Space Telescope; Spectral energy distribution; Flux (metallurgy); Gamma ray; Light curve; Photon; Astronomy; Galaxy; Redshift","score_opus":0.008826358386136896,"score_gpt":0.20656943715708326,"score_spread":0.19774307877094635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105731191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990231,0.00006504492,0.00020697826,0.000038335576,0.0000042780725,0.000012883164,0.00021160934,0.0000092587725,0.00042849872],"genre_scores_gemma":[0.9976305,0.00008112409,0.00047524518,0.00004757329,0.00001963484,0.000014167256,0.0011871916,0.000004966596,0.000539603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997582,0.000029687586,0.000013874871,0.00007342796,0.000079760204,0.000045102734],"domain_scores_gemma":[0.9989299,0.000095461815,0.00035208164,0.00010727627,0.00019879015,0.00031646652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060983165,0.00028102807,0.0002954547,0.0010151768,0.0007890937,0.00043629075,0.0003585566,0.0004781988,0.00037025192],"category_scores_gemma":[0.0007307502,0.00017253176,0.00030060316,0.0007560534,0.00023283307,0.00034769136,0.0006970353,0.00048348092,0.00024778437],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044739814,0.00095833896,0.948464,0.00003736171,0.0001451848,0.0017941168,0.00084024185,0.0008975106,0.026239486,0.00018586745,0.0007129585,0.01927752],"study_design_scores_gemma":[0.000005502652,0.00014612469,0.9977507,0.000002104031,0.000012144301,0.00036173055,0.000098539116,0.00040397295,0.000602305,0.000018822542,0.0005928204,0.00000533016],"about_ca_topic_score_codex":0.0076622698,"about_ca_topic_score_gemma":0.016660547,"teacher_disagreement_score":0.0076622698,"about_ca_system_score_codex":0.00043976097,"about_ca_system_score_gemma":0.0003228924,"threshold_uncertainty_score":0.015235305},"labels":[],"label_agreement":null},{"id":"W2105951587","doi":"10.1088/0004-637x/772/2/145","title":"HIGH-CONTRAST NEAR-INFRARED IMAGING POLARIMETRY OF THE PROTOPLANETARY DISK AROUND RY TAU","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Spectral energy distribution; Infrared; Astrophysics; Radiative transfer; Polarimetry; Protoplanetary disk; Millimeter; Optics; Wavelength; Scattering; Stars","score_opus":0.004543204282020741,"score_gpt":0.2007148534233896,"score_spread":0.19617164914136886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105951587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99721825,0.00012834498,0.0008882731,0.00003415169,0.000004163822,0.000008908823,0.00028276493,0.00008102904,0.0013540795],"genre_scores_gemma":[0.99794036,0.00008534939,0.0014616475,0.000014095071,0.000015720978,0.000005614112,0.00028436803,0.000012510236,0.0001803137],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999629,0.0000041491558,0.0000013875655,0.000009948978,0.000010110762,0.0000114589175],"domain_scores_gemma":[0.99987257,0.000022385679,0.000032428397,0.000018120989,0.00002470005,0.00002978872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008328428,0.00019876784,0.00015500616,0.0005236868,0.00026155938,0.00030765185,0.00024909308,0.00025881082,0.00052301964],"category_scores_gemma":[0.00019843814,0.0001454362,0.00013194821,0.0002817218,0.00017272565,0.00019883513,0.00021199831,0.00023557429,0.00021249149],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011692947,0.00035287865,0.34525374,0.00020617238,0.00017447757,0.00250227,0.001429194,0.022415327,0.58767956,0.001250513,0.0020911365,0.035475448],"study_design_scores_gemma":[0.00006266788,0.00015968992,0.95896745,0.000017689004,0.00006526256,0.00081139355,0.0002060466,0.025664836,0.012404302,0.00029796385,0.0013243236,0.000018384728],"about_ca_topic_score_codex":0.0029510427,"about_ca_topic_score_gemma":0.00364786,"teacher_disagreement_score":0.0029510427,"about_ca_system_score_codex":0.00016699573,"about_ca_system_score_gemma":0.000101911945,"threshold_uncertainty_score":0.0058677793},"labels":[],"label_agreement":null},{"id":"W2105999278","doi":"10.1088/0004-637x/807/1/62","title":"ACCRETION-POWERED PULSATIONS IN AN APPARENTLY QUIESCENT NEUTRON STAR BINARY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":143,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Neutron star; Astrophysics; Millisecond pulsar; Pulsar; Accretion (finance); Astronomy; Luminosity; X-ray binary; X-ray burster; Millisecond; X-ray pulsar; Pulsar planet; Compact star; Binary pulsar; Stars; Stellar evolution; Stellar mass loss","score_opus":0.031846817943381935,"score_gpt":0.2720474249408699,"score_spread":0.240200606997488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2105999278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962866,0.000051448027,0.000043362183,0.000007659765,0.000001167433,0.0000012262511,0.000015990014,0.0000046529376,0.00024585196],"genre_scores_gemma":[0.9996357,0.000043842054,0.00011977908,0.000010998449,0.000007912681,0.000002896226,0.00006821454,0.0000015911867,0.00010904563],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999608,0.000003873173,0.0000051283027,0.000012912141,0.000008473095,0.000008902849],"domain_scores_gemma":[0.9997806,0.00003842257,0.000111163696,0.00001788887,0.000010380402,0.00004148583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012662397,0.00010497633,0.00017890356,0.00038248274,0.00034068973,0.00038039478,0.00018296628,0.0002553227,0.00054896873],"category_scores_gemma":[0.0005124505,0.00010308973,0.00006337081,0.00036429995,0.00027393183,0.0002588027,0.0004912213,0.00020357347,0.0001426402],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011019065,0.00024362087,0.751204,0.00008871999,0.00005233187,0.004701528,0.00096308964,0.00065411127,0.21411179,0.0010786606,0.00037649114,0.025423761],"study_design_scores_gemma":[0.00003517608,0.00029065635,0.9871523,0.000008412498,0.000018981375,0.0036370803,0.00024129602,0.001587262,0.0057343994,0.0006364458,0.0006500544,0.0000079604415],"about_ca_topic_score_codex":0.00065887667,"about_ca_topic_score_gemma":0.00070036296,"teacher_disagreement_score":0.00065887667,"about_ca_system_score_codex":0.00022081869,"about_ca_system_score_gemma":0.0000701178,"threshold_uncertainty_score":0.0018364787},"labels":[],"label_agreement":null},{"id":"W2106324679","doi":"10.1086/511780","title":"An Analysis of the Broadband (22-3900 MHz) Radio Spectrum of HB 3 (G132.7+1.3): The Detection of Thermal Radio Emission from an Evolved Supernova Remnant?","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Bremsstrahlung; Physics; Supernova; Astrophysics; Synchrotron; Radio spectrum; Spectral line; Interstellar medium; Synchrotron radiation; Supernova remnant; Electron; Astronomy; Optics; Galaxy; Nuclear physics","score_opus":0.006206390182237623,"score_gpt":0.22476173799046634,"score_spread":0.21855534780822872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2106324679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904174,0.00012314112,0.00043143058,0.0000092628225,0.0000019255008,0.000002840302,0.00012829171,0.000021675254,0.00023958951],"genre_scores_gemma":[0.99794203,0.00009344269,0.0011884688,0.000024061776,0.0000075115718,0.0000034798686,0.0006007524,0.000013914471,0.00012628913],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999658,0.0000031010636,0.000001733663,0.000009598135,0.0000110171595,0.000008771097],"domain_scores_gemma":[0.9998727,0.000017234112,0.000047904363,0.0000093347135,0.000022895025,0.00002990061],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009461849,0.0002518986,0.00018360154,0.0006426843,0.00014947023,0.00021562577,0.00016276231,0.00022721812,0.00059494644],"category_scores_gemma":[0.00012979373,0.00008280462,0.00027568202,0.00048338808,0.00013670875,0.000088852204,0.00018407975,0.0001777126,0.000203311],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003803795,0.000059066788,0.4049235,0.00009382529,0.00013352443,0.0012914059,0.00025868494,0.0008709008,0.5749424,0.00012219271,0.00024748262,0.016676664],"study_design_scores_gemma":[0.000007499453,0.000086916036,0.99073607,0.000005882735,0.00005032377,0.00069789554,0.00009025916,0.0017036243,0.0060227546,0.0000578416,0.0005333623,0.0000074837567],"about_ca_topic_score_codex":0.0020949945,"about_ca_topic_score_gemma":0.005017649,"teacher_disagreement_score":0.0020949945,"about_ca_system_score_codex":0.00011125338,"about_ca_system_score_gemma":0.000052923206,"threshold_uncertainty_score":0.00416559},"labels":[],"label_agreement":null},{"id":"W2106614505","doi":"10.1088/0004-637x/809/2/132","title":"A COORDINATED X-RAY AND OPTICAL CAMPAIGN OF THE NEAREST MASSIVE ECLIPSING BINARY,<i>δ</i>ORIONIS Aa. I. OVERVIEW OF THE X-RAY SPECTRUM","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Leibniz-Institut für Astrophysik Potsdam; Leibniz-Gemeinschaft; Astrophysics Science Division; Fédération Wallonie-Bruxelles; Universität Potsdam; Oak Ridge Associated Universities; Fonds de recherche du Québec – Nature et technologies; Goddard Space Flight Center; National Science Foundation","keywords":"Physics; Astrophysics; Photosphere; Photometry (optics); Binary number; Spectral line; Line (geometry); Emission spectrum; Astronomy; Stars","score_opus":0.02725792499213105,"score_gpt":0.2496337157502857,"score_spread":0.22237579075815464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2106614505","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9443168,0.0008203344,0.0026733102,0.00015943195,0.00006824542,0.00040615053,0.038025472,0.0005561371,0.012974051],"genre_scores_gemma":[0.89443415,0.0008729732,0.018867685,0.0002644601,0.000207351,0.0003728529,0.07840795,0.00024986317,0.006322588],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970657,0.000031371233,0.000021157193,0.000120438075,0.00006765332,0.00005270821],"domain_scores_gemma":[0.9990951,0.000039518076,0.00019019633,0.00015941847,0.00020946472,0.00030634817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004118801,0.00035630475,0.00036855118,0.0019728257,0.0007519237,0.0007240832,0.00026249196,0.0002607534,0.0020599822],"category_scores_gemma":[0.00039035597,0.00024189427,0.0002765178,0.0015590243,0.00017902677,0.0004988156,0.0008726466,0.00033180427,0.00089605316],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011367217,0.0008338809,0.7465077,0.0005360754,0.00033543684,0.00077567634,0.0016911151,0.0015913766,0.13215412,0.00084540347,0.011884639,0.101707965],"study_design_scores_gemma":[0.0000140952925,0.00013366458,0.98207575,0.00001277437,0.00003252575,0.00019080708,0.00016245252,0.00026621573,0.0022633786,0.00006236394,0.014777173,0.00000887428],"about_ca_topic_score_codex":0.020502,"about_ca_topic_score_gemma":0.05427317,"teacher_disagreement_score":0.020502,"about_ca_system_score_codex":0.0005589403,"about_ca_system_score_gemma":0.00096652773,"threshold_uncertainty_score":0.040765345},"labels":[],"label_agreement":null},{"id":"W2106659600","doi":"10.1088/0004-637x/692/2/1447","title":"ΛCDM SATELLITES AND H I COMPANIONS—THE ARECIBO ALFA SURVEY OF NGC 2903","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Science and Technology Facilities Council","keywords":"Physics; Galaxy; Astrophysics; Milky Way; Astronomy; Dwarf galaxy","score_opus":0.013021789785443237,"score_gpt":0.2261634984147199,"score_spread":0.21314170862927664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2106659600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953519,0.00021967986,0.000049265167,0.00007278379,0.0000049797877,0.0000050766635,0.0012891457,0.000007782313,0.0029994051],"genre_scores_gemma":[0.99704474,0.00029253893,0.00010755421,0.00004675666,0.000013237692,0.000004270236,0.0015080012,0.0000048178463,0.0009781624],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999287,0.000005817885,0.000003035894,0.000016286656,0.000021136502,0.000025123183],"domain_scores_gemma":[0.9997143,0.000015189537,0.00009219007,0.000018920495,0.00005280623,0.000106501655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021788984,0.000119019045,0.0002153252,0.0009864048,0.00056256994,0.0003304752,0.00020467018,0.00013279871,0.0016348346],"category_scores_gemma":[0.00031335198,0.00006998487,0.00009473134,0.0012641167,0.00015061392,0.00021070537,0.00036994249,0.00012635825,0.00034732133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011041302,0.000035340203,0.9810043,0.000019309251,0.000025787993,0.00011216739,0.00059281284,0.00009615353,0.005149242,0.00021939412,0.0021817249,0.010453336],"study_design_scores_gemma":[0.0000019999427,0.000004149858,0.9989864,0.000002041579,0.0000028175803,0.000020232637,0.00012325261,0.000026538873,0.000053234973,0.000013372063,0.00076542574,5.828908e-7],"about_ca_topic_score_codex":0.07656687,"about_ca_topic_score_gemma":0.16633207,"teacher_disagreement_score":0.07656687,"about_ca_system_score_codex":0.00040732042,"about_ca_system_score_gemma":0.00042421522,"threshold_uncertainty_score":0.15224242},"labels":[],"label_agreement":null},{"id":"W2106672187","doi":"10.1088/0004-637x/786/1/29","title":"A LARGE CATALOG OF ACCURATE DISTANCES TO MOLECULAR CLOUDS FROM PS1 PHOTOMETRY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Centre National de la Recherche Scientifique; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Photometry (optics); Molecular cloud; Stars; Line-of-sight; Homogeneous; Systematic error","score_opus":0.0072327225007784894,"score_gpt":0.24950564748405699,"score_spread":0.2422729249832785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2106672187","genre_codex":"empirical","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7394463,0.010832605,0.043206483,0.00050835276,0.00025567567,0.000317039,0.15614298,0.004463852,0.04482678],"genre_scores_gemma":[0.67707646,0.007834858,0.058936905,0.00035262844,0.0005256504,0.00028584624,0.24626784,0.0010859402,0.0076338137],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99826366,0.00010224026,0.0001551609,0.00035934176,0.0010019279,0.00011768567],"domain_scores_gemma":[0.99327034,0.0010719008,0.0012933015,0.0020217341,0.0018169257,0.0005257083],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014321901,0.0005969091,0.00065627554,0.009581746,0.00080827955,0.0014059967,0.00072396424,0.00038959977,0.0052455924],"category_scores_gemma":[0.0060585123,0.00043263665,0.00037261265,0.011834348,0.00029020236,0.0020769048,0.0016258336,0.0005766299,0.004879968],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002303436,0.00016773299,0.48232305,0.0012879823,0.00031158506,0.00040480072,0.0011180151,0.0054816487,0.03413577,0.006838026,0.048338026,0.41936296],"study_design_scores_gemma":[0.00003248343,0.00008836769,0.846267,0.00015881097,0.000103440645,0.0004124767,0.00025985268,0.0024618611,0.008854054,0.002419952,0.13887432,0.00006733567],"about_ca_topic_score_codex":0.0037598049,"about_ca_topic_score_gemma":0.005355609,"teacher_disagreement_score":0.009581746,"about_ca_system_score_codex":0.0006973825,"about_ca_system_score_gemma":0.00093959016,"threshold_uncertainty_score":0.017548263},"labels":[],"label_agreement":null},{"id":"W2106835843","doi":"10.1088/0004-637x/723/2/1736","title":"OPTICAL REDSHIFT AND RICHNESS ESTIMATES FOR GALAXY CLUSTERS SELECTED WITH THE SUNYAEV-Zel'dovich EFFECT FROM 2008 SOUTH POLE TELESCOPE OBSERVATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Jet Propulsion Laboratory; National Institute of Standards and Technology; California Institute of Technology; National Aeronautics and Space Administration; U.S. Department of Energy; Harvard University; National Science Foundation","keywords":"Physics; Redshift; Astrophysics; South Pole Telescope; Galaxy cluster; Galaxy; Telescope; Redshift survey; Sunyaev–Zel'dovich effect; Astronomy; Cosmology; Cluster (spacecraft)","score_opus":0.006247013502676157,"score_gpt":0.20641803761785885,"score_spread":0.2001710241151827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2106835843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99885285,0.000091426424,0.00017900323,0.000009503195,0.0000010365663,0.0000030748286,0.00024995132,0.000013186684,0.00060001237],"genre_scores_gemma":[0.99913836,0.00003218103,0.00018438704,0.0000027682963,0.0000023456325,0.0000021748158,0.00055961736,0.000002888489,0.0000751987],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987483,0.000012205863,0.000007129237,0.00003904803,0.000033127562,0.00003362163],"domain_scores_gemma":[0.99944943,0.00009266465,0.00023456627,0.000057018577,0.00005289429,0.00011339368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019137583,0.00017555631,0.00022734143,0.0015486489,0.0002652212,0.0003680928,0.00020027452,0.00010952112,0.00067444664],"category_scores_gemma":[0.00064011227,0.00014849259,0.00013844116,0.00042142384,0.0002242179,0.00018342113,0.0005389528,0.00009887891,0.000113244096],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008650504,0.000008956431,0.9893311,0.000013781139,0.000036125963,0.00005650666,0.00012703356,0.0010819866,0.0041336096,0.00015838754,0.00029854046,0.0046675033],"study_design_scores_gemma":[0.0000048348734,0.000010292769,0.998659,0.0000020178309,0.0000066941325,0.000036068097,0.000032656055,0.0006352389,0.00034212923,0.000027620687,0.000241178,0.0000022027884],"about_ca_topic_score_codex":0.009015737,"about_ca_topic_score_gemma":0.01837684,"teacher_disagreement_score":0.009015737,"about_ca_system_score_codex":0.00051388226,"about_ca_system_score_gemma":0.00012121284,"threshold_uncertainty_score":0.017926514},"labels":[],"label_agreement":null},{"id":"W2106859358","doi":"10.1088/0004-637x/797/1/27","title":"REVEALING H<sub>2</sub>D<sup>+</sup>DEPLETION AND COMPACT STRUCTURE IN STARLESS AND PROTOSTELLAR CORES WITH ALMA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; National Research Council Canada; University of Victoria; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Protostar; Substructure; Star formation; Hydrostatic equilibrium; Accretion (finance); Ophiuchus; Submillimeter Array","score_opus":0.006219764335754297,"score_gpt":0.2104772793947456,"score_spread":0.20425751505899128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2106859358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991272,0.0000622426,0.00010887848,0.000015220657,0.0000012083569,0.0000028190098,0.00014952828,0.000012041323,0.0005207967],"genre_scores_gemma":[0.99915636,0.000024027384,0.00032034251,0.000024374103,0.000006498896,0.0000031608092,0.00030821055,0.0000034835382,0.00015357704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994516,0.0000036963559,0.0000029306748,0.000017266848,0.000014418108,0.000016479536],"domain_scores_gemma":[0.9997727,0.000025068292,0.00008347503,0.000020878493,0.000027727225,0.0000701922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010357383,0.00012576563,0.000119790784,0.00046365295,0.00026125484,0.00034096852,0.00027202335,0.00022069979,0.0011138179],"category_scores_gemma":[0.00022200131,0.0001170204,0.00011961204,0.0002644014,0.0001872969,0.00017106759,0.0003565972,0.0001583977,0.00019339066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040664474,0.000054228713,0.7814061,0.000042895248,0.000058032176,0.0008038757,0.00035662978,0.0002790482,0.20932186,0.00013169015,0.00036073622,0.0067780945],"study_design_scores_gemma":[0.000005475887,0.000039772996,0.99306715,0.0000021723552,0.000011089365,0.0005011927,0.00008923554,0.0005721064,0.0051803323,0.00004369955,0.00048465305,0.000003064362],"about_ca_topic_score_codex":0.0026826847,"about_ca_topic_score_gemma":0.0055853175,"teacher_disagreement_score":0.0026826847,"about_ca_system_score_codex":0.0002551662,"about_ca_system_score_gemma":0.00008003136,"threshold_uncertainty_score":0.005334139},"labels":[],"label_agreement":null},{"id":"W2106908029","doi":"10.1088/0004-637x/734/1/10","title":"MUSTANG HIGH ANGULAR RESOLUTION SUNYAEV-ZEL'DOVICH EFFECT IMAGING OF SUBSTRUCTURE IN FOUR GALAXY CLUSTERS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Substructure; Sunyaev–Zel'dovich effect; Galaxy cluster; Redshift; Cluster (spacecraft); Angular resolution (graph drawing); Galaxy; Astronomy","score_opus":0.005986533223778689,"score_gpt":0.19568111582042794,"score_spread":0.18969458259664926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2106908029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989459,0.000049706247,0.00013793551,0.000017382828,0.0000011393084,0.0000032445323,0.00015980059,0.000026489603,0.0006584433],"genre_scores_gemma":[0.9988392,0.0000331968,0.000469027,0.00001037788,0.0000047723797,0.0000043209243,0.00033672177,0.000005640973,0.0002966671],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990785,0.0000059620693,0.0000047476856,0.000022913173,0.000019986082,0.00003852852],"domain_scores_gemma":[0.99979347,0.000017888657,0.000046245998,0.00002063674,0.00001850912,0.00010331447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012062192,0.00015888797,0.00015796874,0.0012150077,0.0003248354,0.00042045774,0.00019866115,0.00016400035,0.0012336117],"category_scores_gemma":[0.00016898387,0.0001530388,0.00011907637,0.00039140153,0.00018158459,0.000113264825,0.00059958984,0.00014834767,0.00012226118],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004815324,0.00008250045,0.7514369,0.00006190884,0.00013131349,0.00058777985,0.0009293179,0.0009172297,0.22273172,0.00065089134,0.001203389,0.020785488],"study_design_scores_gemma":[0.000011322933,0.000023534763,0.99675626,0.0000026013133,0.000014001972,0.00012024709,0.00007032504,0.00041962054,0.001910012,0.000047218055,0.0006206427,0.000004232702],"about_ca_topic_score_codex":0.006596799,"about_ca_topic_score_gemma":0.018295217,"teacher_disagreement_score":0.006596799,"about_ca_system_score_codex":0.00027246278,"about_ca_system_score_gemma":0.00013924782,"threshold_uncertainty_score":0.013116837},"labels":[],"label_agreement":null},{"id":"W2107146745","doi":"10.1088/0004-637x/763/2/127","title":"GALAXY CLUSTERS DISCOVERED VIA THE SUNYAEV-ZEL’DOVICH EFFECT IN THE FIRST 720 SQUARE DEGREES OF THE SOUTH POLE TELESCOPE SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":280,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Jet Propulsion Laboratory; Office of Science; McGill University; University of Chicago; Deutsche Forschungsgemeinschaft; Smithsonian Astrophysical Observatory; Massachusetts Institute of Technology; California Institute of Technology; U.S. Department of Energy; Gordon and Betty Moore Foundation; Kavli Institute for Cosmological Physics, University of Chicago; Canada Research Chairs; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Redshift; South Pole Telescope; Galaxy; Galaxy cluster; Telescope; Cluster (spacecraft); Neutrino","score_opus":0.007163314961687948,"score_gpt":0.20283202477588902,"score_spread":0.19566870981420106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2107146745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980038,0.0001582678,0.00006895612,0.000033048924,0.0000039842016,0.0000056058493,0.0005816642,0.00001654486,0.0011281696],"genre_scores_gemma":[0.9986444,0.00009243078,0.00009266864,0.000012330215,0.0000072129706,0.0000044066487,0.00087748165,0.0000039694182,0.00026511034],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996754,0.000021846983,0.0000127729445,0.00007611556,0.00012550234,0.000088453875],"domain_scores_gemma":[0.99916744,0.00007843114,0.00038111175,0.000077528035,0.00007418456,0.00022131753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021723413,0.00014958145,0.00028974895,0.0015136256,0.000493521,0.000578278,0.00021386328,0.00012371421,0.001626473],"category_scores_gemma":[0.0007448512,0.00015357806,0.00014769334,0.000905296,0.00035961714,0.00020791084,0.0007942345,0.00015133113,0.0002993391],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007429859,0.00001368098,0.9909045,0.000016007429,0.00003176249,0.0001397423,0.00025821678,0.00018700336,0.0018361731,0.0001746001,0.001237087,0.0051269126],"study_design_scores_gemma":[0.0000043525797,0.000009571635,0.99897623,0.0000018535563,0.0000047204558,0.000060980863,0.00005509235,0.00007763978,0.00009043632,0.000016732372,0.0007009967,0.0000013212956],"about_ca_topic_score_codex":0.01612995,"about_ca_topic_score_gemma":0.042607006,"teacher_disagreement_score":0.01612995,"about_ca_system_score_codex":0.0006024474,"about_ca_system_score_gemma":0.00034901628,"threshold_uncertainty_score":0.032072127},"labels":[],"label_agreement":null},{"id":"W2107212616","doi":"10.1086/429855","title":"The Sunyaev‐Zel'dovich Effect in CMB‐calibrated Theories Applied to the Cosmic Background Imager Anisotropy Power at<i>l</i>&gt; 2000","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Toronto; University of Alberta; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Physics; Astrophysics; Sunyaev–Zel'dovich effect; Anisotropy; Spectral density; Cosmic background radiation; Anomaly (physics); Amplitude; Optics; Quantum mechanics","score_opus":0.0036630206189171978,"score_gpt":0.23248901303611708,"score_spread":0.2288259924171999,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2107212616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.72948873,0.0052391784,0.1972359,0.01072692,0.0009988986,0.00004812841,0.00030015007,0.00065588736,0.055306166],"genre_scores_gemma":[0.9916083,0.00086848193,0.0040633157,0.00030685338,0.00039429063,0.000017261335,0.00007791628,0.00014818183,0.0025153903],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9992787,0.0002840185,0.000029857038,0.00018423646,0.00011952113,0.0001037037],"domain_scores_gemma":[0.9943896,0.0036954277,0.0005799351,0.0006805026,0.0003516505,0.00030290123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0049670623,0.0006861642,0.0009317554,0.0022032682,0.0011154403,0.0026732795,0.0014391629,0.0014846531,0.0033395658],"category_scores_gemma":[0.017782705,0.0005719428,0.00083054986,0.0011300186,0.0052957,0.0027028273,0.0020249344,0.0019420277,0.00024127397],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000087062464,0.000019297782,0.008490304,0.00006625562,0.00007425282,0.00020445393,0.00031258684,0.02346861,0.00068739237,0.95437044,0.0017927623,0.010426544],"study_design_scores_gemma":[0.00006014708,0.000027244465,0.01899312,0.00005368666,0.00008007104,0.000120147015,0.00017629168,0.10764953,0.0010347966,0.86930245,0.002436732,0.000065757195],"about_ca_topic_score_codex":0.006343915,"about_ca_topic_score_gemma":0.005929498,"teacher_disagreement_score":0.006343915,"about_ca_system_score_codex":0.0016032631,"about_ca_system_score_gemma":0.0010373292,"threshold_uncertainty_score":0.026268661},"labels":[],"label_agreement":null},{"id":"W2107382915","doi":"10.1088/0004-637x/761/2/183","title":"HIGH-REDSHIFT COOL-CORE GALAXY CLUSTERS DETECTED VIA THE SUNYAEV-ZEL'DOVICH EFFECT IN THE SOUTH POLE TELESCOPE SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"South Pole Telescope; Galaxy cluster; Redshift; Cluster (spacecraft); Galaxy; Surface brightness; Brightest cluster galaxy; Telescope","score_opus":0.009973183989593208,"score_gpt":0.2204507643019962,"score_spread":0.210477580312403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2107382915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996208,0.00004520772,0.00006326113,0.00000962661,9.040995e-7,0.0000015780669,0.00009591864,0.0000044209132,0.00015814764],"genre_scores_gemma":[0.99963737,0.000023189332,0.00006456438,0.0000061681926,0.0000039643,0.0000013131099,0.0002249484,0.0000023770094,0.00003618292],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996989,0.00004194509,0.000013461675,0.00009506035,0.00008030522,0.000070350274],"domain_scores_gemma":[0.9986362,0.000223582,0.00057312753,0.0001365187,0.00009275488,0.00033786867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003448057,0.00019095058,0.00040127555,0.0009839874,0.00038980096,0.0005909154,0.0002807284,0.00018377844,0.0007283821],"category_scores_gemma":[0.00118893,0.0001940203,0.00019033182,0.00064492633,0.0006132413,0.00023481992,0.00088720495,0.00021417919,0.000118632895],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008964098,0.000008146464,0.99516654,0.000008437474,0.000046645313,0.000058600974,0.00015703191,0.00012976915,0.0026727,0.000098290744,0.000120829376,0.0014432416],"study_design_scores_gemma":[0.000003492328,0.000008008768,0.9995857,8.707313e-7,0.000006128835,0.00003211862,0.000028502558,0.00010869641,0.00009949937,0.00001572127,0.000110000976,0.000001284823],"about_ca_topic_score_codex":0.0072410027,"about_ca_topic_score_gemma":0.014996551,"teacher_disagreement_score":0.0072410027,"about_ca_system_score_codex":0.00042415838,"about_ca_system_score_gemma":0.00016292505,"threshold_uncertainty_score":0.01439774},"labels":[],"label_agreement":null},{"id":"W2107441581","doi":"10.1088/0004-637x/792/2/133","title":"COSMIC RAY ACCELERATION AT PERPENDICULAR SHOCKS IN SUPERNOVA REMNANTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Cosmic ray; Supernova; Particle acceleration; Momentum (technical analysis); Acceleration; Spectral line; Diffusion; Shock (circulatory); Astrophysics; Computational physics; Spectral index; Momentum diffusion; Particle (ecology); Turbulence; Classical mechanics; Mechanics; Quantum mechanics","score_opus":0.009467436385930878,"score_gpt":0.22247619293870738,"score_spread":0.2130087565527765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2107441581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98497283,0.00017236976,0.009988021,0.00006192979,0.000018225304,0.000015758465,0.000071102324,0.00015338109,0.0045464328],"genre_scores_gemma":[0.99787796,0.00012990746,0.0011104288,0.00001591498,0.000007280296,0.00000895935,0.000078532095,0.000025558107,0.0007454945],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999218,0.000020133686,0.000006411932,0.000015178209,0.000020568652,0.000015836938],"domain_scores_gemma":[0.99975425,0.00005653428,0.00009089374,0.000019670635,0.000030918643,0.000047799484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027904965,0.00037954462,0.0002685302,0.0005327221,0.00027791434,0.0008138601,0.00034526177,0.00033386264,0.0010065569],"category_scores_gemma":[0.0012089043,0.00022735314,0.00043209567,0.0002679006,0.0004120472,0.00035453046,0.0005999411,0.00033755178,0.00016453714],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055966375,0.00021286607,0.06378945,0.00014894754,0.00019219297,0.0017461093,0.00036264514,0.80673677,0.060619842,0.055152662,0.0009531274,0.009525686],"study_design_scores_gemma":[0.000075250726,0.00017445102,0.024015505,0.000019083534,0.000038123355,0.00026964003,0.000096503674,0.9592205,0.0052309837,0.0098751085,0.00094620656,0.00003859206],"about_ca_topic_score_codex":0.0040367544,"about_ca_topic_score_gemma":0.0014799964,"teacher_disagreement_score":0.0040367544,"about_ca_system_score_codex":0.00045516857,"about_ca_system_score_gemma":0.00023928772,"threshold_uncertainty_score":0.00802654},"labels":[],"label_agreement":null},{"id":"W2107889393","doi":"10.1088/0004-637x/756/2/142","title":"A MEASUREMENT OF GRAVITATIONAL LENSING OF THE MICROWAVE BACKGROUND USING SOUTH POLE TELESCOPE DATA","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":267,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Gravitational lens; Weak gravitational lensing; Strong gravitational lensing; Amplitude; Gravitational lensing formalism; Dark matter; Spectral density; Redshift; Galaxy; Optics; Statistics","score_opus":0.059248370459220066,"score_gpt":0.28768906715537806,"score_spread":0.228440696696158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2107889393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.988181,0.000118022435,0.002695978,0.00010117383,0.0000072217567,0.000021777245,0.005205721,0.0001512624,0.0035178636],"genre_scores_gemma":[0.9871683,0.00010004595,0.0033114715,0.000030920637,0.000023429326,0.000018744659,0.00884351,0.000026873538,0.00047656844],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99926895,0.00009873143,0.000034117053,0.00021285168,0.00032063198,0.00006467368],"domain_scores_gemma":[0.9974794,0.0003857316,0.0010638899,0.00037913315,0.00048452645,0.0002073654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006815935,0.00038771093,0.00030057452,0.0015243306,0.00029332613,0.0005536616,0.00034742182,0.0003096003,0.0012784787],"category_scores_gemma":[0.0034206975,0.0002906401,0.00031988873,0.0017485921,0.00024367643,0.00050533254,0.00055968453,0.00029406056,0.0005762208],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016126178,0.00004934076,0.9491148,0.00008434888,0.00023421041,0.00017591524,0.00035495023,0.0030397805,0.02629344,0.0010311373,0.0020765376,0.017384253],"study_design_scores_gemma":[0.000005987988,0.000023007078,0.99299026,0.000004608996,0.000017757175,0.0000674074,0.000022862194,0.0022969448,0.0025610747,0.00011415508,0.001886744,0.000009201193],"about_ca_topic_score_codex":0.012439591,"about_ca_topic_score_gemma":0.020524524,"teacher_disagreement_score":0.012439591,"about_ca_system_score_codex":0.0007555482,"about_ca_system_score_gemma":0.00028771904,"threshold_uncertainty_score":0.024734318},"labels":[],"label_agreement":null},{"id":"W2107917519","doi":"10.1086/586729","title":"A Magellan IMACS Spectroscopic Search for Lyα‐emitting Galaxies at Redshift 5.7","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; St. Mary's University","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy; Astronomy; Luminosity; Population; Emission spectrum; Luminosity function; Quasar; Line (geometry); Spectral line","score_opus":0.013847606936280057,"score_gpt":0.23794460084245797,"score_spread":0.2240969939061779,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2107917519","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99561346,0.000116689065,0.00077722967,0.00006471267,0.000003876349,0.00002956609,0.001717373,0.00016067394,0.001516431],"genre_scores_gemma":[0.9886185,0.00007923358,0.004589698,0.00006569446,0.000018538141,0.00001946638,0.0049784887,0.000017836797,0.001612615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975866,0.000018276993,0.000008164449,0.000070282986,0.00008004271,0.00006443855],"domain_scores_gemma":[0.9990871,0.000060198287,0.00027646456,0.00007537232,0.00016821793,0.00033267948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056153897,0.0002797852,0.00021049875,0.003097277,0.00055680546,0.00031554367,0.00045295942,0.00026703486,0.0023760712],"category_scores_gemma":[0.00048088658,0.00016621905,0.00022066,0.0009571256,0.0001610157,0.00029668174,0.00037056796,0.00015527733,0.0007771038],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001532885,0.00011069275,0.95196265,0.000030447216,0.00005199844,0.00020465588,0.00039143738,0.00020285594,0.019582335,0.0002768083,0.0028881507,0.024144726],"study_design_scores_gemma":[0.000013973267,0.000095511445,0.9932909,0.0000069319026,0.000024050407,0.00019926674,0.00013917711,0.0009198229,0.002348281,0.00006533371,0.0028904865,0.0000062984072],"about_ca_topic_score_codex":0.011956382,"about_ca_topic_score_gemma":0.03414122,"teacher_disagreement_score":0.011956382,"about_ca_system_score_codex":0.000413079,"about_ca_system_score_gemma":0.00041433485,"threshold_uncertainty_score":0.02377361},"labels":[],"label_agreement":null},{"id":"W2107923150","doi":"10.1088/0004-637x/709/1/120","title":"GALACTIC CEPHEIDS WITH<i>SPITZER</i>. I. LEAVITT LAW AND COLORS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Western University","funders":"","keywords":"Cepheid variable; Supergiant; Photometry (optics); Large Magellanic Cloud; Stars; Extinction (optical mineralogy); Galaxy; Variable star","score_opus":0.0062432235224033255,"score_gpt":0.2201084797643023,"score_spread":0.21386525624189898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2107923150","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8655362,0.0045863027,0.006111718,0.000716161,0.000115690375,0.00009133926,0.0037883504,0.0005479127,0.11850635],"genre_scores_gemma":[0.9931431,0.00050883327,0.0011962448,0.00012591996,0.0000455034,0.00002819559,0.001409314,0.000030084546,0.0035128202],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983907,0.000024254367,0.000013123227,0.000046862486,0.000036646376,0.000040122315],"domain_scores_gemma":[0.99905616,0.0001343035,0.0004265544,0.00009648118,0.00013343689,0.0001530692],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017705584,0.0002849977,0.00016348559,0.0010367102,0.00048279448,0.0008092403,0.00030873547,0.0002133598,0.009126168],"category_scores_gemma":[0.0016743946,0.000060982038,0.00012415016,0.0010390205,0.00045203118,0.00040311785,0.0003747767,0.000313019,0.0022777035],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002866475,0.00006909147,0.8970269,0.00009204305,0.000057624835,0.0007143902,0.00068574655,0.00055671873,0.00711298,0.017547237,0.011593221,0.06425742],"study_design_scores_gemma":[0.00001209093,0.00009488076,0.96238637,0.000027818965,0.000018161576,0.0022217233,0.000335314,0.0007439191,0.00069708773,0.0058604158,0.027592016,0.0000101949245],"about_ca_topic_score_codex":0.0035646288,"about_ca_topic_score_gemma":0.0029844434,"teacher_disagreement_score":0.009126168,"about_ca_system_score_codex":0.00031195726,"about_ca_system_score_gemma":0.00014531851,"threshold_uncertainty_score":0.030530035},"labels":[],"label_agreement":null},{"id":"W2108430221","doi":"10.1088/0004-637x/719/2/1045","title":"MEASUREMENTS OF SECONDARY COSMIC MICROWAVE BACKGROUND ANISOTROPIES WITH THE SOUTH POLE TELESCOPE","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":180,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; Office of Science; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Cosmic microwave background; Physics; Astrophysics; South Pole Telescope; Spectral density; Galaxy; Point source; Amplitude; Anisotropy; Cosmology; Cosmic infrared background; Sunyaev–Zel'dovich effect; Cosmic background radiation; Galaxy cluster; Astronomy; Optics","score_opus":0.012495857495238048,"score_gpt":0.2337533643357394,"score_spread":0.22125750684050136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2108430221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9801462,0.000106762185,0.005077686,0.00007463188,0.0000144813575,0.000034583347,0.0033696056,0.00026251262,0.010913521],"genre_scores_gemma":[0.9853833,0.00016526267,0.0062899883,0.000039610764,0.000045193097,0.00003687322,0.005915505,0.000056364643,0.0020679252],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972683,0.000019096718,0.000008554013,0.00007657804,0.00012647337,0.000042409803],"domain_scores_gemma":[0.9993487,0.00006396373,0.00020198718,0.00010343074,0.00015409813,0.00012786445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002454165,0.00040220964,0.0001910934,0.0011529372,0.00029711623,0.00032112442,0.00025646083,0.00018136742,0.002655218],"category_scores_gemma":[0.0006081,0.00022400804,0.00019107769,0.000669748,0.00017851777,0.00027854036,0.00037633945,0.0002848822,0.0010254908],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031718763,0.00008797757,0.84413546,0.00007036185,0.00008780884,0.0003175366,0.00055125117,0.000677265,0.105587184,0.0008829217,0.0039548473,0.043330166],"study_design_scores_gemma":[0.000011614364,0.00007537957,0.9871373,0.0000033237397,0.000016935277,0.00023522004,0.00002925227,0.0012447999,0.0069848867,0.00013700036,0.004114896,0.000009249867],"about_ca_topic_score_codex":0.0028886183,"about_ca_topic_score_gemma":0.009335248,"teacher_disagreement_score":0.0028886183,"about_ca_system_score_codex":0.00025642585,"about_ca_system_score_gemma":0.000109995235,"threshold_uncertainty_score":0.008882582},"labels":[],"label_agreement":null},{"id":"W2108732492","doi":"10.1088/0004-637x/710/2/1694","title":"OBSERVATIONS AND MODELING OF RELATIVISTIC SPIN PRECESSION IN PSR J1141–6545","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Pulsar; Position angle; Astrophysics; Polarization (electrochemistry); Precession; Angular momentum; Computational physics; Astronomy; Classical mechanics; Galaxy","score_opus":0.028861332009535813,"score_gpt":0.3532510937607056,"score_spread":0.3243897617511698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2108732492","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996944,0.00017957091,0.0016734977,0.00006288137,0.000006755222,0.000008767054,0.00011900989,0.000120111676,0.0008854238],"genre_scores_gemma":[0.99910694,0.00005843404,0.000526027,0.000008811448,0.0000053586427,0.000003931272,0.00017207804,0.000016512333,0.00010194528],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987864,0.000023204975,0.000010584208,0.000034566277,0.000028380888,0.00002456618],"domain_scores_gemma":[0.9997359,0.00005576442,0.0000997686,0.000036866928,0.000031097155,0.000040628718],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043049533,0.0003470173,0.00034430114,0.00059257186,0.00031417518,0.00073020963,0.00062671094,0.00037612388,0.000379403],"category_scores_gemma":[0.0009672108,0.00031854754,0.000453901,0.0005645544,0.0002596249,0.00031407663,0.00034755963,0.0002848363,0.00015087497],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057115883,0.00024592777,0.5398151,0.00012515002,0.00029341158,0.0008990699,0.0006838911,0.3807947,0.048428588,0.0031866375,0.0011716401,0.023784647],"study_design_scores_gemma":[0.00007384076,0.00014237416,0.40397614,0.000013377895,0.000069357055,0.00020907518,0.00008998148,0.5905612,0.0026603092,0.00078565505,0.0013680104,0.00005061241],"about_ca_topic_score_codex":0.016642496,"about_ca_topic_score_gemma":0.009941158,"teacher_disagreement_score":0.016642496,"about_ca_system_score_codex":0.0011379605,"about_ca_system_score_gemma":0.00034684667,"threshold_uncertainty_score":0.033091307},"labels":[],"label_agreement":null},{"id":"W2108966901","doi":"10.1088/0004-637x/749/1/45","title":"CHARACTERIZATION OF TURBULENCE FROM SUBMILLIMETER DUST EMISSION","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Western University","funders":"","keywords":"Turbulence; Physics; Anisotropy; Polarization (electrochemistry); Stokes parameters; Magnetic field; Computational physics; Astrophysics; Scattering; Optics; Meteorology; Quantum mechanics; Chemistry","score_opus":0.011500748308830668,"score_gpt":0.22665114614646298,"score_spread":0.21515039783763232,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2108966901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97739923,0.0004054509,0.020547567,0.000044429915,0.000022806395,0.000012226981,0.00021630658,0.000092547634,0.0012594606],"genre_scores_gemma":[0.9955492,0.00013904898,0.0037755657,0.000013435516,0.000021286323,0.000006468835,0.0002998215,0.0000127207695,0.00018237613],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999373,0.0000061810692,0.0000027822107,0.000013667148,0.000021355998,0.00001879844],"domain_scores_gemma":[0.99985063,0.00004113785,0.000040740782,0.000012658552,0.000027416521,0.000027354261],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010794925,0.00019558404,0.00013846385,0.000690179,0.00019660773,0.00033610823,0.00015682331,0.00010675708,0.00034514428],"category_scores_gemma":[0.00039580715,0.00011070805,0.00017252946,0.00028415336,0.00013621637,0.00030433404,0.00020307755,0.00023396712,0.00008336962],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035870477,0.000084562584,0.29714024,0.00010725924,0.00007982994,0.0005349084,0.00025717323,0.006234223,0.6332263,0.0038867828,0.0003790309,0.057711035],"study_design_scores_gemma":[0.000025074381,0.00012241607,0.84461015,0.000019412806,0.000035244695,0.00050524523,0.0001354875,0.06631463,0.083526276,0.0023972655,0.0022665784,0.00004225247],"about_ca_topic_score_codex":0.0011361197,"about_ca_topic_score_gemma":0.0016264793,"teacher_disagreement_score":0.0011361197,"about_ca_system_score_codex":0.00018244488,"about_ca_system_score_gemma":0.0001472838,"threshold_uncertainty_score":0.002259016},"labels":[],"label_agreement":null},{"id":"W2109100416","doi":"10.1088/0004-637x/783/2/93","title":"COMPARING SIMULATED EMISSION FROM MOLECULAR CLOUDS USING EXPERIMENTAL DESIGN","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Molecular cloud; Magnetohydrodynamic drive; Principal component analysis; Mach number; Magnetic field; Field (mathematics); Adiabatic process; Sample (material); Magnetohydrodynamics","score_opus":0.029161345339738923,"score_gpt":0.27419554538135243,"score_spread":0.24503420004161353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109100416","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78801924,0.00007761113,0.20942676,0.00012954428,0.00008702128,0.00052386016,0.00058254,0.00026169664,0.00089176773],"genre_scores_gemma":[0.94110847,0.000025345194,0.05689095,0.00007170869,0.000022787855,0.0008444999,0.00086909765,0.000035811034,0.00013139118],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9892019,0.0078092907,0.00056524423,0.001270156,0.00085823465,0.0002951814],"domain_scores_gemma":[0.92718256,0.053586204,0.005773972,0.009501064,0.0033740473,0.0005821189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.016598813,0.00068468077,0.00060189987,0.00083888054,0.00056171906,0.0012624322,0.001456563,0.0011225776,0.0008035965],"category_scores_gemma":[0.0628533,0.00045165495,0.0013664061,0.0006409208,0.0017701953,0.0010301818,0.001512252,0.0009911064,0.00009743133],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0036871228,0.0021778997,0.08872838,0.0003585574,0.0011395343,0.0001610443,0.0005993796,0.8082294,0.019563612,0.02930271,0.0007820038,0.045270294],"study_design_scores_gemma":[0.00054762186,0.0043558287,0.026251528,0.00002902388,0.00018414643,0.000087050415,0.00021335339,0.91374445,0.022671258,0.030169804,0.0016091528,0.0001367972],"about_ca_topic_score_codex":0.0013068614,"about_ca_topic_score_gemma":0.0009631353,"teacher_disagreement_score":0.016598813,"about_ca_system_score_codex":0.0014034222,"about_ca_system_score_gemma":0.00085051503,"threshold_uncertainty_score":0.08778393},"labels":[],"label_agreement":null},{"id":"W2109131429","doi":"10.1088/0004-637x/779/2/92","title":"LONG TERM OBSERVATIONS OF B2 1215+30 WITH VERITAS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; National Research Foundation; Space Telescope Science Institute; Smithsonian Institution; Science Foundation Ireland; National Science Foundation","keywords":"Blazar; Physics; Astrophysics; Spectral energy distribution; BL Lac object; MAGIC (telescope); Fermi Gamma-ray Space Telescope; Flux (metallurgy); Spectral index; Gamma ray; Spectral line; Astronomy; Galaxy","score_opus":0.012308095226038908,"score_gpt":0.2096885180740724,"score_spread":0.1973804228480335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109131429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936033,0.00030510387,0.00076975924,0.00004623531,0.000016001826,0.00001713536,0.0015915975,0.0002121893,0.0034386998],"genre_scores_gemma":[0.99054915,0.00011410046,0.0015948573,0.000046773755,0.000034093046,0.000016472946,0.006579537,0.000046404228,0.0010185761],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996357,0.000024032814,0.000012689586,0.00009575045,0.00014542128,0.000086526175],"domain_scores_gemma":[0.9992872,0.00004913653,0.00024332295,0.00009084392,0.00012772362,0.00020180551],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000535707,0.00034422762,0.00034761347,0.0010205508,0.0005751802,0.00065737765,0.00053881336,0.00039373303,0.0015016526],"category_scores_gemma":[0.0005499277,0.0003008632,0.0003299441,0.0009016649,0.0002691877,0.0004318906,0.00083562796,0.0005282414,0.00061448663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015579952,0.00046569383,0.68676525,0.0003049774,0.0004987589,0.0017768666,0.0013288966,0.008210188,0.22523576,0.0019248436,0.0067177946,0.06521295],"study_design_scores_gemma":[0.00006002128,0.00037727956,0.97604024,0.00003105997,0.000076865304,0.00061048806,0.00015364289,0.0053415103,0.006317966,0.00021830852,0.010731277,0.000041437455],"about_ca_topic_score_codex":0.012277311,"about_ca_topic_score_gemma":0.02906332,"teacher_disagreement_score":0.012277311,"about_ca_system_score_codex":0.0011055846,"about_ca_system_score_gemma":0.00037585615,"threshold_uncertainty_score":0.024411678},"labels":[],"label_agreement":null},{"id":"W2109140604","doi":"10.1086/588018","title":"The Multiwavelength Survey by Yale‐Chile (MUSYC): Wide<i>K</i>‐Band Imaging, Photometric Catalogs, Clustering, and Physical Properties of Galaxies at<i>z</i> ∼ 2","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; York University","funders":"","keywords":"Galaxy; Redshift; Observatory; Cosmic variance; Star formation; Telescope; Correlation function (quantum field theory); Luminous infrared galaxy; Spatial correlation","score_opus":0.01066458143801181,"score_gpt":0.20200805861010926,"score_spread":0.19134347717209746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109140604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8663753,0.0011351436,0.0029976894,0.0002566997,0.000030792668,0.00018095822,0.09357089,0.0005516185,0.034900907],"genre_scores_gemma":[0.8530052,0.00095744047,0.010640266,0.0002178426,0.000045686986,0.0002836,0.12060338,0.0002188567,0.014027823],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999138,0.000008958514,0.000004546644,0.000026257716,0.000025073,0.000021451371],"domain_scores_gemma":[0.99960285,0.000020129992,0.00012843845,0.000053678745,0.00005473741,0.00014016479],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017994357,0.00022949249,0.0001676537,0.0014330524,0.00029299437,0.00039983523,0.00028988434,0.0001143783,0.0044032475],"category_scores_gemma":[0.0002809825,0.00019701007,0.00013316695,0.0015132683,0.00014089746,0.00025042993,0.0007522334,0.00023132973,0.0009893945],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034743015,0.00013616114,0.82646745,0.00026694572,0.0001521835,0.00032455256,0.00094942044,0.0010913843,0.028950576,0.0022864814,0.06455236,0.07447498],"study_design_scores_gemma":[0.000012516605,0.000008879776,0.9816798,0.000017907676,0.000009090223,0.0001085775,0.000104845734,0.00025742888,0.0008158408,0.000057649788,0.016920447,0.00000703861],"about_ca_topic_score_codex":0.067640916,"about_ca_topic_score_gemma":0.11168454,"teacher_disagreement_score":0.067640916,"about_ca_system_score_codex":0.00052573514,"about_ca_system_score_gemma":0.0005703094,"threshold_uncertainty_score":0.13449436},"labels":[],"label_agreement":null},{"id":"W2109148012","doi":"10.1088/0004-637x/736/1/61","title":"IMPROVED CONSTRAINTS ON COSMIC MICROWAVE BACKGROUND SECONDARY ANISOTROPIES FROM THE COMPLETE 2008 SOUTH POLE TELESCOPE DATA","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cosmic microwave background; South Pole Telescope; Spectral density; Amplitude; Cosmic background radiation; Estimator; Anisotropy; Telescope","score_opus":0.039374509451750486,"score_gpt":0.2507137400230927,"score_spread":0.21133923057134224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109148012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878539,0.000114790455,0.002684864,0.00012190293,0.00000810228,0.000011864734,0.0064646383,0.00018398177,0.0025559862],"genre_scores_gemma":[0.9716441,0.000098706936,0.005554482,0.000054739216,0.000038866736,0.000039946906,0.022021657,0.00007918129,0.00046824236],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994642,0.00007299652,0.000031458556,0.00012443453,0.00023625602,0.000070649985],"domain_scores_gemma":[0.9981363,0.00030039428,0.0004990971,0.0005023064,0.00037182463,0.00019001089],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072803267,0.000555097,0.000567657,0.0017062918,0.00027405433,0.0005635851,0.0004798819,0.000259569,0.001928586],"category_scores_gemma":[0.0025898656,0.00037794854,0.00050088915,0.0011143311,0.00017651594,0.00038612692,0.0007500041,0.00043870814,0.0009049101],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036179565,0.000086370725,0.88957906,0.00016500444,0.00021869005,0.00034642764,0.00043745726,0.007767678,0.052889645,0.0013233752,0.007357857,0.039466593],"study_design_scores_gemma":[0.000023631657,0.000029867202,0.98540133,0.000009518641,0.00004103495,0.00012347635,0.000029068293,0.007637543,0.0025055103,0.0003208159,0.0038647142,0.000013496036],"about_ca_topic_score_codex":0.004458582,"about_ca_topic_score_gemma":0.009574043,"teacher_disagreement_score":0.004458582,"about_ca_system_score_codex":0.00044473936,"about_ca_system_score_gemma":0.0002896012,"threshold_uncertainty_score":0.008865237},"labels":[],"label_agreement":null},{"id":"W2109306534","doi":"10.1088/0004-637x/740/2/71","title":"DETECTIONS OF FAINT Lyα EMITTERS AT<i>z</i>= 5.7: GALAXY BUILDING BLOCKS AND ENGINES OF REIONIZATION","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; St. Mary's University","funders":"","keywords":"Reionization; Physics; Galaxy; Astrophysics; Flux (metallurgy); Astronomy; Telescope; Hubble Deep Field; Population; Redshift","score_opus":0.008064544049842536,"score_gpt":0.19330101274351122,"score_spread":0.1852364686936687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109306534","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99556607,0.00024527323,0.0015489442,0.00007185592,0.000006477835,0.000008037315,0.00031579635,0.00007702981,0.0021604514],"genre_scores_gemma":[0.9954163,0.00011704553,0.0031134936,0.00009124048,0.000014671442,0.0000059589497,0.00059576804,0.000015121581,0.00063032494],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998468,0.0000070342858,0.000004706877,0.00004359454,0.000048440066,0.000049482827],"domain_scores_gemma":[0.999607,0.000037895086,0.00013421323,0.000048505128,0.00007862243,0.00009372561],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032074473,0.00024503144,0.00027050238,0.00047387395,0.00038338333,0.0007458495,0.00043883364,0.00035134985,0.0015350349],"category_scores_gemma":[0.00032870268,0.0001932762,0.00023643342,0.00025951726,0.00024854412,0.0004328588,0.0005878869,0.0004773083,0.0006297886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042400323,0.000101146004,0.70209754,0.00010543078,0.000105834646,0.0005475679,0.0007760456,0.00040598703,0.25059882,0.0015031855,0.0016151059,0.04171939],"study_design_scores_gemma":[0.000019588324,0.0002458109,0.93337935,0.000026833985,0.00011541049,0.0012676861,0.00039622543,0.0017770297,0.054998968,0.00084488036,0.0068997513,0.00002848791],"about_ca_topic_score_codex":0.0011861823,"about_ca_topic_score_gemma":0.0027908233,"teacher_disagreement_score":0.0015350349,"about_ca_system_score_codex":0.00020574125,"about_ca_system_score_gemma":0.00011040654,"threshold_uncertainty_score":0.0051351786},"labels":[],"label_agreement":null},{"id":"W2109343995","doi":"10.1086/421313","title":"Deep CCD Surface Photometry of Galaxy Clusters. II. Searching for Intracluster Starlight in Non‐cD clusters","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Intracluster medium; Galaxy cluster; Brightest cluster galaxy; Astronomy; Photometry (optics); Abell 2744; Galaxy; Galaxy merger; Cluster (spacecraft); Galaxy groups and clusters; Elliptical galaxy; Stars","score_opus":0.0070241335759013415,"score_gpt":0.23032202484508366,"score_spread":0.2232978912691823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109343995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99388313,0.00006561026,0.00053222646,0.000015141173,0.0000030142687,0.000012631466,0.003121319,0.000056976387,0.0023099978],"genre_scores_gemma":[0.991941,0.000037836853,0.0012551468,0.000011517445,0.0000043178893,0.000010811985,0.005763597,0.0000094748775,0.00096618646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983287,0.000013854949,0.000008402762,0.000039691706,0.00005159504,0.00005358511],"domain_scores_gemma":[0.9995427,0.000050744282,0.00012576085,0.00006714433,0.00007821451,0.00013550455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014984969,0.0001853441,0.00018257105,0.0013800589,0.0003556776,0.00029798687,0.00024728876,0.00016203128,0.0026879022],"category_scores_gemma":[0.0005500126,0.00012450345,0.00012854002,0.0009605551,0.0001494252,0.00016371443,0.0004342245,0.00011204259,0.0008371641],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013240002,0.00004228801,0.9605632,0.000039105988,0.00003146669,0.00007556253,0.00021126855,0.0010686937,0.024096692,0.0003389083,0.0014442363,0.011956048],"study_design_scores_gemma":[0.0000029625317,0.000013407977,0.9973762,0.0000012737644,0.0000040507757,0.000076472345,0.000051646308,0.0005167565,0.000989998,0.000060176924,0.00090449024,0.0000025805184],"about_ca_topic_score_codex":0.013991774,"about_ca_topic_score_gemma":0.029348763,"teacher_disagreement_score":0.013991774,"about_ca_system_score_codex":0.00054144696,"about_ca_system_score_gemma":0.00020157687,"threshold_uncertainty_score":0.027820647},"labels":[],"label_agreement":null},{"id":"W2109496206","doi":"10.1086/309115","title":"Solar System Tests of Higher Dimensional Gravity","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Tests of general relativity; Precession; General relativity; Apsidal precession; Schwarzschild metric; Geodesy; Nutation; Ephemeris; Astrophysics; Classical mechanics; Astronomy; Satellite; Planet; Geology; Gravitational redshift","score_opus":0.005642709538145687,"score_gpt":0.23303260969944942,"score_spread":0.22738990016130373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109496206","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90499806,0.0007687462,0.0060782274,0.00094471447,0.00012452257,0.000045671277,0.0019371476,0.00013557036,0.08496737],"genre_scores_gemma":[0.9971727,0.00009795374,0.0009381462,0.000083866464,0.00006140824,0.000020132366,0.0007115215,0.0000071379754,0.00090698525],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99753404,0.0013127512,0.00014809896,0.0002958319,0.000515638,0.00019374506],"domain_scores_gemma":[0.9874824,0.0051661064,0.0026617497,0.0024000488,0.0012763921,0.0010132785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028394756,0.0005225958,0.00036477746,0.0014752356,0.0005677985,0.0012730185,0.0007269778,0.0003784921,0.009676969],"category_scores_gemma":[0.010721255,0.00009202188,0.00049092807,0.0014116431,0.0020810736,0.001412025,0.0022418129,0.00051035255,0.00058493833],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016969902,0.0003980404,0.41567692,0.0003352701,0.00054911344,0.00045463818,0.0025161717,0.009262279,0.0057454007,0.49064726,0.007453346,0.06526455],"study_design_scores_gemma":[0.00032920853,0.0012800752,0.7129651,0.000070713395,0.000100900244,0.0004876215,0.0014634582,0.011919039,0.0032444512,0.24919453,0.018843891,0.00010099093],"about_ca_topic_score_codex":0.0018197239,"about_ca_topic_score_gemma":0.0009401208,"teacher_disagreement_score":0.009676969,"about_ca_system_score_codex":0.00069177686,"about_ca_system_score_gemma":0.00032953135,"threshold_uncertainty_score":0.032372653},"labels":[],"label_agreement":null},{"id":"W2109527936","doi":"10.1086/588777","title":"Composition of Ices in Low‐Mass Extrasolar Planets","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Natural Resources Canada","funders":"","keywords":"Planetesimal; Planet; Exoplanet; Astrobiology; Planetary migration; Protoplanetary disk; Physics; Planetary mass; Astrophysics; Terrestrial planet; Gravitational microlensing; Carbon fibers; Materials science; Stars","score_opus":0.00842524695933347,"score_gpt":0.20241667637048946,"score_spread":0.193991429411156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109527936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938285,0.00014552253,0.00020603582,0.000004906208,5.773771e-7,7.76499e-7,0.000046522702,0.000004990269,0.00020782533],"genre_scores_gemma":[0.99951935,0.000084426814,0.00020588815,0.0000016913381,0.0000011835367,8.88161e-7,0.0001228417,0.0000030258143,0.000060687238],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99997365,0.0000033088575,0.0000017609244,0.000009740886,0.0000043540344,0.0000071219633],"domain_scores_gemma":[0.9998727,0.0000276407,0.00005437965,0.000011628156,0.000014640579,0.000018971867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005591947,0.00014056882,0.00013451323,0.00067891926,0.00019652545,0.00032765677,0.0001364712,0.00013313064,0.00035158335],"category_scores_gemma":[0.0002685115,0.0000799675,0.00013310614,0.00028187438,0.00021506914,0.0002451714,0.00018268614,0.0000865655,0.000088251734],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039623457,0.000057316065,0.6954911,0.000112349415,0.000104083454,0.00038237814,0.00033130724,0.025421383,0.26319978,0.0008380318,0.00014968918,0.0135164065],"study_design_scores_gemma":[0.000035950827,0.00015606382,0.8637557,0.000016540258,0.0000758731,0.000633444,0.00032887032,0.07397089,0.05774679,0.0013210457,0.0019425846,0.000016282567],"about_ca_topic_score_codex":0.0020860059,"about_ca_topic_score_gemma":0.0017748686,"teacher_disagreement_score":0.0020860059,"about_ca_system_score_codex":0.00018466919,"about_ca_system_score_gemma":0.00007495858,"threshold_uncertainty_score":0.0041477084},"labels":[],"label_agreement":null},{"id":"W2109528201","doi":"10.1088/0004-637x/805/2/187","title":"A MISSING-LINK IN THE SUPERNOVA–GRB CONNECTION: THE CASE OF SN 2012ap","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Gamma-ray burst; Supernova; Ejecta; Outflow; Redshift; Light curve; Baryon; Pair-instability supernova","score_opus":0.02716656263618882,"score_gpt":0.2647861972955098,"score_spread":0.23761963465932096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109528201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97552365,0.0021043564,0.0051553,0.004030946,0.00021402662,0.000034383826,0.0004026069,0.00006214824,0.01247265],"genre_scores_gemma":[0.99680436,0.0005408592,0.0011646722,0.00015920897,0.00021809069,0.0000099664585,0.00022566564,0.000016844571,0.00086040143],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992372,0.00016897371,0.00008396334,0.00021792811,0.000114685405,0.00017719544],"domain_scores_gemma":[0.9960848,0.0017321634,0.00085616007,0.0006170764,0.00024113353,0.00046864848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014039176,0.00034842137,0.00049039087,0.0015856706,0.0021594535,0.002217441,0.0007922854,0.002746436,0.0045904894],"category_scores_gemma":[0.0075498843,0.00024033539,0.00054402475,0.0018808453,0.0017964363,0.002625963,0.0021233945,0.002324729,0.0006357836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090955826,0.0002959966,0.68225926,0.00020208598,0.00019311355,0.19501366,0.0033900163,0.001796104,0.0025459125,0.053191956,0.0045414595,0.055660903],"study_design_scores_gemma":[0.00014152363,0.00031546212,0.35340768,0.0004485477,0.0006726323,0.42073017,0.012133476,0.023175647,0.0028945354,0.14285272,0.04301178,0.00021578421],"about_ca_topic_score_codex":0.0032633846,"about_ca_topic_score_gemma":0.0025053583,"teacher_disagreement_score":0.0045904894,"about_ca_system_score_codex":0.0004371579,"about_ca_system_score_gemma":0.00058325985,"threshold_uncertainty_score":0.0153567195},"labels":[],"label_agreement":null},{"id":"W2109574122","doi":"10.1088/0004-637x/765/2/153","title":"ON THE DIFFERENT ANALYTICAL RESULTS OBTAINED FOR THE PARALLEL DIFFUSION COEFFICIENT OF COSMIC PARTICLES WITH ADIABATIC FOCUSING","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Adiabatic process; Diffusion; Magnetic field; COSMIC cancer database; Field (mathematics); Particle (ecology); Computational physics; Statistical physics; Classical mechanics; Astrophysics; Thermodynamics; Quantum mechanics","score_opus":0.01114240460127675,"score_gpt":0.22386496619993712,"score_spread":0.21272256159866038,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109574122","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.10986779,0.024052305,0.7420945,0.0024757036,0.0009901568,0.00012358106,0.00023503888,0.00039994236,0.119760945],"genre_scores_gemma":[0.82730037,0.040794104,0.09902829,0.001518915,0.0017471847,0.00019224029,0.00033349707,0.00066901714,0.028416436],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99946076,0.0001584316,0.000036340844,0.00011082979,0.00016070125,0.000072918476],"domain_scores_gemma":[0.9976532,0.0013737897,0.00028858302,0.000211296,0.00037140623,0.000101738326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013199308,0.0014049761,0.0007962552,0.0025001075,0.0007429219,0.0010404498,0.0013330956,0.0008382921,0.0024202194],"category_scores_gemma":[0.00727294,0.00033061512,0.0014812027,0.0012153903,0.002104316,0.0023369796,0.0012882254,0.0019173824,0.00069344515],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000751474,0.00007707326,0.0008274177,0.00076317997,0.00007648142,0.0007653998,0.000566929,0.0635236,0.01389858,0.8941262,0.0026318636,0.022668183],"study_design_scores_gemma":[0.00002801499,0.000066003566,0.0022414315,0.000338346,0.00014684995,0.0015077268,0.00019502011,0.48870906,0.014786632,0.47954723,0.012223482,0.00021019431],"about_ca_topic_score_codex":0.001902292,"about_ca_topic_score_gemma":0.0013455874,"teacher_disagreement_score":0.0025001075,"about_ca_system_score_codex":0.0010507245,"about_ca_system_score_gemma":0.00064476527,"threshold_uncertainty_score":0.0080964565},"labels":[],"label_agreement":null},{"id":"W2109622958","doi":"10.1088/0004-637x/802/1/61","title":"CHARACTERIZATION OF LOW-MASS, WIDE-SEPARATION SUBSTELLAR COMPANIONS TO STARS IN UPPER SCORPIUS: NEAR-INFRARED PHOTOMETRY AND SPECTROSCOPY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Stantec (Canada)","funders":"","keywords":"Photometry (optics); Brown dwarf; Stars; Spectroscopy; Spectral line; Stellar classification; Atmosphere (unit); Effective temperature","score_opus":0.01252663163667492,"score_gpt":0.24817946619425513,"score_spread":0.2356528345575802,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109622958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994742,0.000036027486,0.00010719785,0.0000045949982,4.1467064e-7,0.0000018831182,0.00004523132,0.0000127931435,0.00031780094],"genre_scores_gemma":[0.9990085,0.00004063708,0.00041516917,0.0000050627827,0.000002175257,0.000002526157,0.00027741655,0.000004311414,0.0002442535],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999455,0.0000033234446,0.0000033084864,0.000019339326,0.000012784793,0.00001576223],"domain_scores_gemma":[0.9998035,0.000016531883,0.00007993065,0.000017621407,0.000023376275,0.000059044844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014821986,0.00021932178,0.00014037084,0.0007520632,0.00034299234,0.00040551947,0.00019415964,0.00018229603,0.0007679595],"category_scores_gemma":[0.00030812618,0.00012181908,0.00012369062,0.0004168573,0.0002484169,0.00025326188,0.0005656263,0.00016712141,0.0002272957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000064436674,0.00003141162,0.95121145,0.000025433541,0.00001719735,0.00039900813,0.00059691386,0.00033107892,0.03796453,0.00011771639,0.00011043508,0.009130474],"study_design_scores_gemma":[0.0000013754559,0.000020449845,0.9980971,0.0000027553424,0.0000048039224,0.00018334542,0.00010011914,0.00037701998,0.0009776339,0.000017478189,0.0002166064,0.0000013152219],"about_ca_topic_score_codex":0.0040923334,"about_ca_topic_score_gemma":0.008678935,"teacher_disagreement_score":0.0040923334,"about_ca_system_score_codex":0.0002076418,"about_ca_system_score_gemma":0.00015038173,"threshold_uncertainty_score":0.008137047},"labels":[],"label_agreement":null},{"id":"W2109710257","doi":"10.1088/0004-637x/719/2/1244","title":"A NEW METHOD FOR OBTAINING THE STAR FORMATION LAW IN GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Star formation; Astrophysics; Physics; Galaxy; Power law; Molecular cloud; Law; Statistics; Mathematics","score_opus":0.010626302091484414,"score_gpt":0.25601539514109733,"score_spread":0.24538909304961293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109710257","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.007784068,0.00024814674,0.9842473,0.000079223566,0.00007359532,0.00007681526,0.00065262686,0.0018821645,0.0049561406],"genre_scores_gemma":[0.14616604,0.0004781015,0.84074086,0.0001953219,0.00028794506,0.0005288559,0.0019446461,0.0009979174,0.008660317],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990884,0.00016681773,0.00005864292,0.0002855446,0.0003475593,0.000053052267],"domain_scores_gemma":[0.9983462,0.00048909674,0.00018583078,0.00059024076,0.00030495072,0.00008377343],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00085474865,0.000598983,0.0006059446,0.0048779054,0.0005454071,0.0018823212,0.0012811403,0.00058251485,0.005711502],"category_scores_gemma":[0.005192451,0.00046365563,0.0009735322,0.0021884984,0.00080298446,0.0017450758,0.0013562422,0.001187591,0.003128292],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000083204024,0.00011995602,0.037560754,0.00032295779,0.00020742438,0.00027322583,0.0010214451,0.018894633,0.029676506,0.2701548,0.0094630495,0.6322222],"study_design_scores_gemma":[0.0001194281,0.00023181149,0.07331672,0.00013323511,0.0000947067,0.001286757,0.0003183064,0.41159698,0.021864722,0.29172912,0.1991033,0.00020489897],"about_ca_topic_score_codex":0.0040586223,"about_ca_topic_score_gemma":0.002725465,"teacher_disagreement_score":0.005711502,"about_ca_system_score_codex":0.0007367448,"about_ca_system_score_gemma":0.00050839,"threshold_uncertainty_score":0.019106865},"labels":[],"label_agreement":null},{"id":"W2109712829","doi":"10.1088/0004-637x/812/1/79","title":"THE EXTREME ULTRAVIOLET DEFICIT: JET CONNECTION IN THE QUASAR 1442+101","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Quasar; Extreme ultraviolet lithography; Extreme ultraviolet; Redshift; Supermassive black hole; Jet (fluid); Flux (metallurgy); Spectral line","score_opus":0.02774733335533929,"score_gpt":0.24196112443845316,"score_spread":0.21421379108311386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109712829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99867684,0.00015193505,0.00022327149,0.00003343234,0.0000026784376,0.0000014611073,0.000040978182,0.0000049512228,0.0008643828],"genre_scores_gemma":[0.99975616,0.000037987043,0.00005602948,0.000008922844,0.000009280264,8.506182e-7,0.00004309507,0.0000014305785,0.00008615854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999436,0.0000065507597,0.0000030674696,0.000018271767,0.000013290077,0.000015222464],"domain_scores_gemma":[0.99966955,0.00006372977,0.0001803289,0.000016325908,0.000013640105,0.0000564817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001850801,0.00015982382,0.0002448502,0.0007139705,0.00019908402,0.00080190634,0.00020240812,0.000291209,0.0008820969],"category_scores_gemma":[0.0005353323,0.000072917726,0.00014877661,0.0007766715,0.00036807556,0.0004230891,0.00038558012,0.00033774754,0.00007802646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025689142,0.000110336325,0.96127826,0.000042423424,0.00007171011,0.0014030338,0.00030898702,0.001581334,0.023941396,0.0023729627,0.00017228661,0.008460507],"study_design_scores_gemma":[0.0000022191618,0.00003247293,0.99816906,0.0000018183198,0.000008886126,0.0002543392,0.000092796414,0.00080393854,0.00026196742,0.00024491514,0.00012457564,0.0000028930804],"about_ca_topic_score_codex":0.0023879248,"about_ca_topic_score_gemma":0.002618362,"teacher_disagreement_score":0.0023879248,"about_ca_system_score_codex":0.00025710423,"about_ca_system_score_gemma":0.00010868331,"threshold_uncertainty_score":0.004748106},"labels":[],"label_agreement":null},{"id":"W2109777103","doi":"10.1088/0004-637x/706/1/119","title":"THE COLLISIONAL DIVOT IN THE KUIPER BELT SIZE DISTRIBUTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; RADIUS; Power law; Astrophysics; Accretion (finance); Distribution (mathematics); Astronomy","score_opus":0.005116353519068483,"score_gpt":0.21628515535599704,"score_spread":0.21116880183692857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109777103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.985109,0.0001306321,0.007572768,0.00012984588,0.00000922039,0.0000139515605,0.0001348679,0.00013351407,0.0067660324],"genre_scores_gemma":[0.9982122,0.000044590764,0.0010619201,0.000021674947,0.0000029951,0.000009311083,0.000113861075,0.000039103594,0.0004942901],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998839,0.000017686367,0.0000039133515,0.000027991062,0.000033338816,0.00003313254],"domain_scores_gemma":[0.9993704,0.00026184836,0.00012443674,0.00007358626,0.000094793686,0.000074894204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003056323,0.00022721358,0.00021810227,0.0003346657,0.0004946768,0.00081978674,0.0007939031,0.00039893595,0.0015175721],"category_scores_gemma":[0.0028636735,0.00029600254,0.00034600697,0.00032851598,0.00056411955,0.0008015923,0.0005429317,0.00046903503,0.00023261207],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033111317,0.00009321444,0.19009602,0.000072139774,0.00006645523,0.0011749347,0.0007698179,0.74299544,0.019868594,0.028004207,0.0013703426,0.015157754],"study_design_scores_gemma":[0.00006447341,0.000065961576,0.060764875,0.000014995114,0.000021616741,0.00039999845,0.00023737554,0.9241348,0.005523233,0.005969414,0.002764126,0.000039144135],"about_ca_topic_score_codex":0.0063420064,"about_ca_topic_score_gemma":0.002934811,"teacher_disagreement_score":0.0063420064,"about_ca_system_score_codex":0.001123754,"about_ca_system_score_gemma":0.00038014445,"threshold_uncertainty_score":0.012610137},"labels":[],"label_agreement":null},{"id":"W2109783508","doi":"10.1086/345986","title":"Galaxy Clustering Evolution in the UH8K Weak‐Lensing Fields","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Galaxy; Redshift; Cluster analysis; Correlation function (quantum field theory); Field galaxy; Redshift survey; Population; Galaxy formation and evolution; Cluster (spacecraft)","score_opus":0.008830573072778151,"score_gpt":0.2147599369538614,"score_spread":0.20592936388108324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109783508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99925953,0.000016769327,0.00008040737,0.0000070532424,3.9504266e-7,0.0000011945,0.00019604087,0.000009790608,0.00042884322],"genre_scores_gemma":[0.9992551,0.000010523475,0.00009691394,0.0000034361658,0.0000013462444,0.0000015598936,0.0004482843,0.0000025832157,0.00018018282],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983156,0.000019694644,0.000007048542,0.000048081896,0.000040396913,0.000053242828],"domain_scores_gemma":[0.9990313,0.000141712,0.00032155574,0.00010154644,0.00017094756,0.00023297564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030519642,0.00020336123,0.00020234945,0.0011820203,0.00026877274,0.00043207777,0.00024804886,0.0001295825,0.0010483643],"category_scores_gemma":[0.0010939289,0.00015149542,0.00011967227,0.00057806034,0.00033773255,0.00024943933,0.00037036242,0.00015382736,0.00020710973],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022481833,0.000038549057,0.970794,0.000018121074,0.00006081936,0.00009921186,0.00027216825,0.0032804783,0.013758488,0.00055481377,0.00051907246,0.010379402],"study_design_scores_gemma":[0.000002266604,0.000013265486,0.9980925,0.0000016369108,0.000004579561,0.000020341391,0.00003112792,0.0012174656,0.0004426867,0.000043921442,0.00012674642,0.0000034503296],"about_ca_topic_score_codex":0.032562155,"about_ca_topic_score_gemma":0.03310567,"teacher_disagreement_score":0.032562155,"about_ca_system_score_codex":0.0011500458,"about_ca_system_score_gemma":0.00018024477,"threshold_uncertainty_score":0.06474525},"labels":[],"label_agreement":null},{"id":"W2109860978","doi":"10.1086/380117","title":"On the Flux of Extrasolar Dust in Earth’s Atmosphere","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Meteoroid; Debris disk; Exoplanet; Astronomy; Interplanetary dust cloud; Astrophysics; Solar System; Stars; Planetary system; Cosmic dust; Astrobiology; Planet; Atmosphere (unit); Interplanetary medium; Debris; Flux (metallurgy); Interplanetary spaceflight; Solar wind; Plasma; Meteorology","score_opus":0.007384473076499251,"score_gpt":0.19731157373807265,"score_spread":0.1899271006615734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2109860978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97199774,0.0032567515,0.001886344,0.0007822531,0.00009071719,0.000009991913,0.0022776925,0.000084952815,0.019613462],"genre_scores_gemma":[0.992428,0.0020169972,0.0010104601,0.000104381346,0.0002569313,0.000008492955,0.0016607617,0.000022377559,0.0024915263],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999923,0.000014060422,0.0000036941035,0.000020943615,0.000025968655,0.000012375402],"domain_scores_gemma":[0.99910176,0.000621154,0.000083062485,0.00003269771,0.00011500081,0.000046396075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025245736,0.00024736446,0.00017721223,0.0012292408,0.00022496074,0.00048405112,0.00023640702,0.00047234652,0.004109539],"category_scores_gemma":[0.0013132534,0.000098158824,0.00013711804,0.00063968473,0.00026874276,0.0006845127,0.00024164576,0.00019997207,0.0006911752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006626272,0.00016723342,0.77794147,0.000489931,0.00014667501,0.00091641466,0.0003293786,0.01379685,0.035346877,0.011603569,0.0127858315,0.14581311],"study_design_scores_gemma":[0.000016342661,0.00005212851,0.9751976,0.000081283964,0.00003090716,0.000372135,0.00009511437,0.010180225,0.0030929085,0.0034237385,0.0074492875,0.000008331952],"about_ca_topic_score_codex":0.0024185046,"about_ca_topic_score_gemma":0.0018395537,"teacher_disagreement_score":0.004109539,"about_ca_system_score_codex":0.00048353348,"about_ca_system_score_gemma":0.00005841625,"threshold_uncertainty_score":0.013747752},"labels":[],"label_agreement":null},{"id":"W2110133807","doi":"10.1088/0004-637x/702/2/1502","title":"LENTICULAR GALAXIES AND THEIR ENVIRONMENTS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Lenticular galaxy; Elliptical galaxy; Galaxy; Flattening; Galaxy cluster; Galaxy group; Peculiar galaxy; Luminosity; Luminous infrared galaxy","score_opus":0.0050477008711760675,"score_gpt":0.18596874538580194,"score_spread":0.18092104451462587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110133807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93562603,0.002153083,0.00074221555,0.000243345,0.000011128642,0.000015344365,0.0003131625,0.000090420406,0.060805283],"genre_scores_gemma":[0.9962992,0.00030856708,0.00021918923,0.00005112671,0.000012546321,0.0000035564115,0.00019670457,0.000010889377,0.0028981434],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998054,0.000039472732,0.0000075542525,0.000036565652,0.00003337953,0.00007769778],"domain_scores_gemma":[0.9993223,0.00006440219,0.00015510932,0.000054240252,0.000070860384,0.0003330788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002615746,0.00016258952,0.00013550761,0.0013274666,0.00092950446,0.0025252467,0.0005893186,0.00020539176,0.0065275785],"category_scores_gemma":[0.0008468465,0.00009642157,0.0000659705,0.0010879558,0.0013046216,0.0007180626,0.0018998095,0.00022454778,0.000815959],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043738986,0.00014992307,0.6654936,0.00014069685,0.00006568357,0.0017299616,0.0128491735,0.0005000773,0.0056291763,0.19478667,0.0063167484,0.11190088],"study_design_scores_gemma":[0.00005197896,0.00017268815,0.82197475,0.00012222497,0.000041882216,0.0024449064,0.012159797,0.0008345681,0.0008249938,0.050653998,0.110680155,0.000038135393],"about_ca_topic_score_codex":0.0061042383,"about_ca_topic_score_gemma":0.005596048,"teacher_disagreement_score":0.0065275785,"about_ca_system_score_codex":0.00081761373,"about_ca_system_score_gemma":0.0003259802,"threshold_uncertainty_score":0.021836936},"labels":[],"label_agreement":null},{"id":"W2110155166","doi":"10.1088/0004-637x/790/1/78","title":"IRRADIATION INSTABILITY AT THE INNER EDGES OF ACCRETION DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Instability; Physics; Opacity; Astrophysics; Irradiation; Accretion (finance); BETA (programming language); Mechanics; Optics; Nuclear physics","score_opus":0.011361486607925141,"score_gpt":0.23704209337359383,"score_spread":0.2256806067656687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110155166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98512787,0.00034976605,0.008230186,0.00006455599,0.000006800441,0.000008188282,0.000051156414,0.0001822356,0.005979189],"genre_scores_gemma":[0.9984261,0.00006502162,0.00097130466,0.000015431284,0.000005522844,0.0000052157798,0.000043135246,0.000018086976,0.00045021102],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999275,0.000008836862,0.0000038813564,0.000019346522,0.000019945537,0.00002046936],"domain_scores_gemma":[0.99930465,0.00021789421,0.00030554668,0.000035949444,0.0000799333,0.000055959863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010335255,0.00018078729,0.00017393577,0.0004383716,0.00033470846,0.0007483121,0.0003859889,0.0002745591,0.0011939132],"category_scores_gemma":[0.000857209,0.0001470475,0.00019278716,0.00016421535,0.00043739154,0.00042214736,0.00057118415,0.00037103757,0.00033650643],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051979825,0.00008990061,0.107983015,0.00028074405,0.00005580316,0.0019310784,0.0018480859,0.06628573,0.76662505,0.010555615,0.0015065421,0.042318646],"study_design_scores_gemma":[0.000058156143,0.00037299655,0.17772974,0.00010429275,0.00005685134,0.0026711076,0.00063695596,0.46220794,0.34048238,0.008432009,0.007164474,0.00008298148],"about_ca_topic_score_codex":0.00088170904,"about_ca_topic_score_gemma":0.00042898435,"teacher_disagreement_score":0.0011939132,"about_ca_system_score_codex":0.00036324534,"about_ca_system_score_gemma":0.00014892763,"threshold_uncertainty_score":0.0039940476},"labels":[],"label_agreement":null},{"id":"W2110226683","doi":"10.1088/0004-637x/744/2/139","title":"COLLISIONAL EVOLUTION OF ULTRA-WIDE TRANS-NEPTUNIAN BINARIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"National Science Foundation","keywords":"Physics; Eccentricity (behavior); Solar System; Population; Binary number; Trans-Neptunian object; Astrophysics; Orbit (dynamics); Mass ratio; Astronomy; Aerospace engineering","score_opus":0.012247885539546956,"score_gpt":0.1954056429413698,"score_spread":0.18315775740182286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110226683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982566,0.00005286825,0.00048288322,0.000041439307,0.000002672734,0.0000032282396,0.00002958324,0.000010514423,0.001120322],"genre_scores_gemma":[0.999516,0.000024248842,0.00016712883,0.000012454386,0.0000013478422,0.0000028098464,0.000046284957,0.0000063747543,0.0002234267],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992764,0.000017173794,0.000004025739,0.000017185164,0.000013201037,0.000020660602],"domain_scores_gemma":[0.99950826,0.00017091,0.000108516266,0.000030475308,0.000041668834,0.00014015473],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033552473,0.0001916702,0.00031661164,0.00036856593,0.001072459,0.0008375915,0.0006872205,0.0003658848,0.0012667467],"category_scores_gemma":[0.0014781837,0.00029779572,0.00026226157,0.00040324294,0.0006823773,0.0007756903,0.00089609285,0.000488126,0.0001693489],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004477941,0.00028039375,0.29817578,0.00005753462,0.00024596392,0.001350471,0.0010614992,0.6563272,0.01647221,0.015889453,0.0011113902,0.008580282],"study_design_scores_gemma":[0.00010595009,0.00020231857,0.12532708,0.000018352079,0.0000697466,0.00041279008,0.0006517282,0.86495155,0.002715424,0.0042527225,0.0012395221,0.00005274358],"about_ca_topic_score_codex":0.013397204,"about_ca_topic_score_gemma":0.012723241,"teacher_disagreement_score":0.013397204,"about_ca_system_score_codex":0.0015776467,"about_ca_system_score_gemma":0.00041853008,"threshold_uncertainty_score":0.026638448},"labels":[],"label_agreement":null},{"id":"W2110402261","doi":"10.1086/497060","title":"Testing LMC Microlensing Scenarios: The Discrimination Power of the SuperMACHO Microlensing Survey","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Impact of Light on Environment and Health","field":"Environmental Science","cited_by":214,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Lawrence Livermore National Laboratory; National Science Foundation; James S. McDonnell Foundation; U.S. Department of Energy; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; Harvard University","keywords":"Gravitational microlensing; Physics; Stars; Large Magellanic Cloud; Astrophysics; Luminosity; Luminosity function; Lens (geology); Astronomy; Galaxy; Optics","score_opus":0.0212604798535689,"score_gpt":0.2449410913015138,"score_spread":0.2236806114479449,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110402261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99740905,0.000044239325,0.0014057251,0.00014867897,0.000002134946,0.000016485781,0.0001318907,0.000023866076,0.0008179029],"genre_scores_gemma":[0.9978846,0.000022992854,0.0017426613,0.00004233989,0.00000353017,0.000007658443,0.00022466942,0.000008122376,0.000063367836],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99842393,0.00090264395,0.00004936338,0.00026194315,0.00020428635,0.00015790119],"domain_scores_gemma":[0.9878055,0.008843679,0.0012267091,0.00085669174,0.00051225675,0.0007552964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.006110661,0.0004928791,0.0005552571,0.00062741706,0.0005602006,0.0012168498,0.0012746067,0.0010666761,0.0005439638],"category_scores_gemma":[0.016895339,0.00032979788,0.0007422574,0.00058449805,0.0009409152,0.0018515713,0.0011307008,0.00054456503,0.00012223239],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001169431,0.00016621068,0.5914817,0.000095749354,0.00044559853,0.00032163248,0.00034409433,0.3820266,0.00474017,0.005470775,0.00066876155,0.013069261],"study_design_scores_gemma":[0.00017343224,0.00041085287,0.13413988,0.000025793033,0.00007821282,0.00017470033,0.00024323282,0.85900164,0.0025075336,0.0027703254,0.00040554593,0.000068840876],"about_ca_topic_score_codex":0.01259983,"about_ca_topic_score_gemma":0.009355126,"teacher_disagreement_score":0.01259983,"about_ca_system_score_codex":0.0010008352,"about_ca_system_score_gemma":0.00056352443,"threshold_uncertainty_score":0.032316685},"labels":[],"label_agreement":null},{"id":"W2110456780","doi":"10.1086/588543","title":"SANEPIC: A Mapmaking Method for Time Stream Data from Large Arrays","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Scientific Research and Discoveries","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Computer science; Pixel; Detector; Algorithm; Noise (video); Covariance matrix; Artificial intelligence; Image (mathematics)","score_opus":0.05170237996089939,"score_gpt":0.34256352201565204,"score_spread":0.29086114205475266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110456780","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0014204239,0.000034472392,0.99428284,0.000035885056,0.00003438522,0.00003975964,0.00037646832,0.003206353,0.0005694616],"genre_scores_gemma":[0.01759764,0.00006655406,0.9786809,0.000046298606,0.000059633585,0.0001379294,0.0013418434,0.000936722,0.0011323781],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9988096,0.0001806862,0.00007243722,0.00029505455,0.0005345698,0.000107738735],"domain_scores_gemma":[0.99656725,0.001240847,0.00026043397,0.00088602246,0.0008872065,0.00015825748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020598304,0.0011494494,0.0011967226,0.0024707327,0.0012038047,0.002388611,0.002595885,0.000998792,0.007503394],"category_scores_gemma":[0.0107369805,0.0010942494,0.0016493127,0.0033339695,0.0006783417,0.0020862175,0.0025863885,0.002327376,0.0041750907],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033356395,0.000095926895,0.0040533147,0.00033921094,0.00023319274,0.0003985208,0.00045385593,0.08645327,0.016020834,0.032923672,0.030550981,0.82814366],"study_design_scores_gemma":[0.0001041167,0.000050253377,0.0021267137,0.00003930577,0.00005263923,0.00040921784,0.0001355102,0.87065315,0.022305302,0.04842991,0.05557917,0.00011473892],"about_ca_topic_score_codex":0.0046235477,"about_ca_topic_score_gemma":0.007757842,"teacher_disagreement_score":0.007503394,"about_ca_system_score_codex":0.0005878051,"about_ca_system_score_gemma":0.002297585,"threshold_uncertainty_score":0.025101364},"labels":[],"label_agreement":null},{"id":"W2110523830","doi":"10.1088/0004-637x/809/2/128","title":"A CHEMICAL TROMPE-L’ŒIL: NO IRON SPREAD IN THE GLOBULAR CLUSTER M22","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Ejecta; Stars; Spectral line; Cluster (spacecraft); Star cluster; Abundance (ecology); Supernova; Ionization; Astronomy; Ion; Quantum mechanics","score_opus":0.01369100735731704,"score_gpt":0.23047841527279633,"score_spread":0.2167874079154793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110523830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997689,0.00003250293,0.000023319846,0.0000046118485,3.443706e-7,4.4895083e-7,0.000036677087,0.0000040890054,0.00012918907],"genre_scores_gemma":[0.9997187,0.000013069469,0.00004201583,0.0000028724573,0.0000016747068,9.2643575e-7,0.00013310683,0.0000020448865,0.000085623724],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999021,0.000006407784,0.000003544933,0.000043467964,0.000018025934,0.000026414837],"domain_scores_gemma":[0.9997912,0.000019191722,0.00004712704,0.000031671083,0.000034475852,0.00007637256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010007268,0.00025574246,0.00022891969,0.00090979424,0.0004313105,0.00048695257,0.00025432414,0.00035251386,0.0006574227],"category_scores_gemma":[0.00034043845,0.00010053179,0.00014563077,0.00059064035,0.00030755828,0.00017577726,0.00043057476,0.00010304885,0.00024973464],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032403,0.000034217894,0.9248522,0.000027611755,0.00006933543,0.0006496051,0.00066644076,0.0010815993,0.06614163,0.00013720771,0.00020878566,0.0058072866],"study_design_scores_gemma":[0.0000037011125,0.000035505902,0.99706215,0.0000015275886,0.000008753103,0.00018766221,0.00016212104,0.00096729887,0.0012845945,0.000030441923,0.00025251674,0.0000036879737],"about_ca_topic_score_codex":0.008755563,"about_ca_topic_score_gemma":0.010836553,"teacher_disagreement_score":0.008755563,"about_ca_system_score_codex":0.00044248413,"about_ca_system_score_gemma":0.00014766827,"threshold_uncertainty_score":0.017409205},"labels":[],"label_agreement":null},{"id":"W2110530179","doi":"10.1086/343764","title":"Density and Velocity Structure of the Be Star Equatorial Disk in the Binary LS I +61o303, a Probable Microquasar","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Neutron star; RADIUS; Accretion (finance); Eddington luminosity; X-ray binary; Radial velocity; Luminosity; Galaxy; Stars","score_opus":0.014729802703944212,"score_gpt":0.21173794001416804,"score_spread":0.19700813731022382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110530179","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99882275,0.00007019355,0.00025800918,0.000021823686,0.000001047447,0.0000019511228,0.000035621382,0.000005919383,0.00078259537],"genre_scores_gemma":[0.9994234,0.000040583687,0.00027220513,0.000008174392,0.00000200445,0.0000030537112,0.000081216276,0.0000031051627,0.00016635757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995685,0.000005161795,0.0000030414017,0.000015417976,0.000011091413,0.000008344356],"domain_scores_gemma":[0.9998317,0.000021077449,0.00006946473,0.000014018076,0.000029816234,0.000033948065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014957474,0.00010465529,0.0002013886,0.00039270514,0.0003139099,0.00039366394,0.00019546397,0.00018863604,0.0005364852],"category_scores_gemma":[0.00045929608,0.00012633778,0.00009313829,0.0002842449,0.00026614906,0.00019284966,0.000332767,0.00015120361,0.00020479549],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032216878,0.00004887419,0.85541785,0.000053501477,0.000029628376,0.0007018322,0.00081647607,0.003463908,0.124928914,0.0020224114,0.00028997706,0.011904478],"study_design_scores_gemma":[0.000010981657,0.00009589097,0.9873696,0.000008486153,0.000015104388,0.00036601158,0.00035270114,0.0077858623,0.0029553124,0.0003460373,0.0006844114,0.000009545534],"about_ca_topic_score_codex":0.0055352408,"about_ca_topic_score_gemma":0.0065909424,"teacher_disagreement_score":0.0055352408,"about_ca_system_score_codex":0.00031443257,"about_ca_system_score_gemma":0.00014730025,"threshold_uncertainty_score":0.011006057},"labels":[],"label_agreement":null},{"id":"W2110531893","doi":"10.1088/0004-637x/789/1/75","title":"<i>NuSTAR</i>OBSERVATIONS OF THE MAGNETAR 1E 2259+586","year":2014,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Outflow; Supernova; Pulsar; Position angle; Spectral line; Neutron star; Pulse (music); Range (aeronautics)","score_opus":0.016631064204815065,"score_gpt":0.28387674100936877,"score_spread":0.2672456768045537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110531893","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950223,0.00027365886,0.0007472879,0.000044139015,0.000016222886,0.0000075347934,0.00095118233,0.0001054364,0.0028321438],"genre_scores_gemma":[0.99362236,0.00014168974,0.0025882341,0.00004935778,0.000039092763,0.000008110306,0.0025968605,0.000020468604,0.0009338388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999318,0.0000040822483,0.0000045174047,0.000019273146,0.000026806592,0.000013430134],"domain_scores_gemma":[0.99973553,0.000013758328,0.00010295972,0.0000328065,0.000041772855,0.000073115276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014728746,0.00017298803,0.00024752063,0.00073028484,0.00027634753,0.00027234902,0.00023428744,0.00017437116,0.00083898526],"category_scores_gemma":[0.00026845315,0.000113020025,0.00016932774,0.00033602637,0.0001378033,0.00016652871,0.000382058,0.00025250626,0.00043110846],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096993014,0.00027937742,0.4798091,0.0002704472,0.00022583653,0.0018099387,0.00042625045,0.0012290804,0.45418617,0.0005155649,0.0033382268,0.056940082],"study_design_scores_gemma":[0.000018106124,0.0002660942,0.98031956,0.000012611936,0.00004801575,0.0016686516,0.00004398322,0.00075855904,0.010476434,0.00012388002,0.0062500783,0.000014014003],"about_ca_topic_score_codex":0.00088045566,"about_ca_topic_score_gemma":0.004302255,"teacher_disagreement_score":0.00088045566,"about_ca_system_score_codex":0.0001143735,"about_ca_system_score_gemma":0.00007601566,"threshold_uncertainty_score":0.0028067231},"labels":[],"label_agreement":null},{"id":"W2110568033","doi":"10.1088/0004-637x/789/1/72","title":"<i>NuSTAR</i>STUDY OF HARD X-RAY MORPHOLOGY AND SPECTROSCOPY OF PWN G21.5–0.9","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar wind nebula; Nebula; Supernova; Spectroscopy; Supernova remnant; Pulsar; Scaling; Particle acceleration; Emission spectrum","score_opus":0.006999320560466329,"score_gpt":0.21907586067497575,"score_spread":0.21207654011450944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110568033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808925,0.00014704031,0.00035613135,0.000022760834,0.0000033017525,0.000003717461,0.00016259945,0.000045293214,0.0011697874],"genre_scores_gemma":[0.9979133,0.000076509736,0.00088523387,0.000030970208,0.000008037839,0.0000045629154,0.00068475964,0.000015358233,0.00038112083],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994934,0.000004191311,0.000003793336,0.000018557768,0.000014126868,0.000009882422],"domain_scores_gemma":[0.9996896,0.000025078974,0.00011694175,0.00004503994,0.000048601796,0.00007480996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001759738,0.00017590904,0.00018781729,0.0008220796,0.00026861086,0.00041461538,0.0002174146,0.00022513968,0.0006138386],"category_scores_gemma":[0.00032390366,0.00011221538,0.00021899476,0.00040082211,0.00021213401,0.00025240588,0.00039994845,0.00021731369,0.00024105413],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003664662,0.00011891494,0.6728962,0.00010296974,0.00015240525,0.0015240788,0.00049341173,0.0011744025,0.30198038,0.0003653276,0.0007718747,0.020053497],"study_design_scores_gemma":[0.0000031642062,0.00007372449,0.99252397,0.0000043816513,0.000013480549,0.00080866256,0.000050990373,0.00057087233,0.005054264,0.000062401115,0.0008290771,0.000005112606],"about_ca_topic_score_codex":0.0010119186,"about_ca_topic_score_gemma":0.002168802,"teacher_disagreement_score":0.0010119186,"about_ca_system_score_codex":0.00019203662,"about_ca_system_score_gemma":0.000062288644,"threshold_uncertainty_score":0.0020534992},"labels":[],"label_agreement":null},{"id":"W2110634338","doi":"10.1088/0004-637x/785/1/47","title":"AN ADAPTIVE OPTICS MULTIPLICITY CENSUS OF YOUNG STARS IN UPPER SCORPIUS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal","funders":"","keywords":"Physics; Stars; Multiplicity (mathematics); Astrophysics; Telescope; Astronomy; Stellar mass; Star formation","score_opus":0.013055758322346223,"score_gpt":0.2337866620870366,"score_spread":0.22073090376469037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110634338","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992607,0.0000465638,0.00015122454,0.0000050057265,4.3893786e-7,0.000002835614,0.00018964731,0.000012478249,0.00033098803],"genre_scores_gemma":[0.99728024,0.00008141969,0.00069610914,0.0000063324837,0.0000050803274,0.0000056855474,0.0015841527,0.000008608212,0.00033237247],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997532,0.000017214576,0.00001893468,0.00008436912,0.000071615985,0.00005470989],"domain_scores_gemma":[0.9989869,0.00011935059,0.0003926435,0.00009789678,0.00014118421,0.00026192566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029595627,0.00023224553,0.00022286449,0.0031813793,0.00044897295,0.0004956009,0.0002675563,0.00016674561,0.00094709604],"category_scores_gemma":[0.0009603382,0.00019033308,0.00020083366,0.0014994387,0.00037829913,0.00039946454,0.0009975586,0.00016325862,0.00029547248],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005908332,0.000017037899,0.9797458,0.000015547368,0.000024035953,0.00015437407,0.0002868236,0.00028985832,0.00880936,0.00007545659,0.00013972855,0.010382899],"study_design_scores_gemma":[0.000001305318,0.00002226826,0.99839896,0.0000023257494,0.000005766362,0.00019595331,0.000069579524,0.00036094576,0.00057303044,0.00002971108,0.00033779806,0.000002336144],"about_ca_topic_score_codex":0.0059449766,"about_ca_topic_score_gemma":0.008952467,"teacher_disagreement_score":0.0059449766,"about_ca_system_score_codex":0.00032750936,"about_ca_system_score_gemma":0.00023647244,"threshold_uncertainty_score":0.011820734},"labels":[],"label_agreement":null},{"id":"W2110870471","doi":"10.1086/519015","title":"The Long‐Period, Massive Binaries HD 37366 and HD 54662: Potential Targets for Long‐Baseline Optical Interferometry","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Spectral line; Binary star; Stars; Interferometry; Binary number; Angular diameter; Astronomical spectroscopy; Light curve; Absorption (acoustics)","score_opus":0.008193516863055904,"score_gpt":0.2385669865346173,"score_spread":0.2303734696715614,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110870471","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986848,0.0002126731,0.0002799609,0.000028342001,0.0000036836507,0.0000048816546,0.00020580887,0.000020541991,0.0005592971],"genre_scores_gemma":[0.99796945,0.00005415262,0.0011587554,0.000012357775,0.000009320455,0.0000036523,0.00062323787,0.0000041832036,0.00016483509],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998729,0.000012644295,0.000004941793,0.00003671758,0.00003123369,0.00004158632],"domain_scores_gemma":[0.9995708,0.00004316,0.00015164903,0.00003385684,0.00003785467,0.00016262165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036737658,0.00037942274,0.00043908344,0.001113392,0.00084684126,0.0005755309,0.00045421722,0.00029276233,0.00088479434],"category_scores_gemma":[0.00043007897,0.00022095094,0.00019661074,0.0010591575,0.0002754012,0.00037432552,0.0006383206,0.00027376186,0.0003152298],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008130419,0.00016517837,0.8661744,0.000060404094,0.000103126324,0.0004283155,0.00031457664,0.0019745308,0.10393942,0.0009867363,0.0007042353,0.024336046],"study_design_scores_gemma":[0.000044153516,0.00016324974,0.98194396,0.0000095286005,0.000060896244,0.00043238708,0.00025897258,0.005899447,0.008987205,0.00063255767,0.0015487338,0.000018818702],"about_ca_topic_score_codex":0.0047770967,"about_ca_topic_score_gemma":0.011003795,"teacher_disagreement_score":0.0047770967,"about_ca_system_score_codex":0.0005928808,"about_ca_system_score_gemma":0.00023980984,"threshold_uncertainty_score":0.009498596},"labels":[],"label_agreement":null},{"id":"W2110906056","doi":"10.1088/0004-637x/693/2/1484","title":"DARK BURSTS IN THE<i>SWIFT</i>ERA: THE PALOMAR 60 INCH-<i>SWIFT</i>EARLY OPTICAL AFTERGLOW CATALOG","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"U.S. Naval Observatory; University of Leicester; California Institute of Technology; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration","keywords":"Swift; Afterglow; Gamma-ray burst; Astrophysics; Physics; Photometry (optics); Optical telescope; Telescope; Galaxy; Astronomy; Extinction (optical mineralogy); Stars; Optics","score_opus":0.007163289504334339,"score_gpt":0.22188565353099113,"score_spread":0.2147223640266568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2110906056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98841876,0.0001670031,0.0004231415,0.000064159685,0.000021901928,0.000021032407,0.006559362,0.000112820024,0.00421178],"genre_scores_gemma":[0.9611933,0.0003781113,0.0021335213,0.00012580035,0.00010637551,0.000035163896,0.03410477,0.000056576802,0.0018664553],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999887,0.0000061245173,0.000014336019,0.000030834344,0.0000322135,0.000029589706],"domain_scores_gemma":[0.9990306,0.00005594894,0.0004704403,0.00013814427,0.00012442244,0.00018045802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027230073,0.00015916971,0.00017342174,0.0022386014,0.00021569015,0.00059399934,0.00024377194,0.00010587871,0.0015824293],"category_scores_gemma":[0.00066957576,0.00012212776,0.000111296984,0.0013061558,0.000128872,0.00038126067,0.0007762926,0.0001462913,0.0005703429],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014989603,0.00007185865,0.9484268,0.000047573412,0.000028791623,0.00037686373,0.0003469733,0.00024586174,0.0042920955,0.00038747166,0.0075889835,0.038036797],"study_design_scores_gemma":[0.000007899981,0.000021539474,0.991699,0.0000074824907,0.000010656754,0.000293632,0.000080464764,0.00025374684,0.0005798554,0.00008157009,0.0069599347,0.000004163569],"about_ca_topic_score_codex":0.005247215,"about_ca_topic_score_gemma":0.0098556755,"teacher_disagreement_score":0.005247215,"about_ca_system_score_codex":0.00012971231,"about_ca_system_score_gemma":0.00016566005,"threshold_uncertainty_score":0.010433316},"labels":[],"label_agreement":null},{"id":"W2111345995","doi":"10.1088/0004-637x/702/1/39","title":"SHOCK-GENERATED VORTICITY IN THE INTERSTELLAR MEDIUM AND THE ORIGIN OF THE STELLAR INITIAL MASS FUNCTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Interstellar medium; Shock wave; Turbulence; Molecular cloud; Stars; Blast wave; Vorticity; Scaling; Spectral density; Shock (circulatory)","score_opus":0.013270486741114387,"score_gpt":0.24352281151783425,"score_spread":0.23025232477671986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111345995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9884798,0.00036153322,0.0075362716,0.00015671141,0.000017538656,0.0000056235644,0.000042667838,0.000047619207,0.0033521494],"genre_scores_gemma":[0.999271,0.00010411731,0.00030861155,0.000007335366,0.000005383353,0.0000015363948,0.000014826568,0.000004674213,0.0002826016],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99997544,0.0000051890574,0.0000011597137,0.000003631688,0.000006806059,0.0000078060875],"domain_scores_gemma":[0.99987626,0.00003277312,0.000041726096,0.0000073922624,0.000014931129,0.000026989741],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009389182,0.0001712179,0.00014715115,0.000373618,0.00030410432,0.0007277788,0.00025803223,0.00031073255,0.0005489269],"category_scores_gemma":[0.0006816666,0.00015044455,0.00016653318,0.0002130303,0.0006353771,0.00051271194,0.0005145496,0.00044277083,0.00010985184],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002446807,0.000119649165,0.056741722,0.00010408186,0.00008319151,0.0035911766,0.00066952774,0.60804695,0.10552046,0.21131846,0.0009468075,0.012613279],"study_design_scores_gemma":[0.00004283639,0.00011842235,0.053336896,0.000027305801,0.000017957844,0.00034702456,0.00023723433,0.9039083,0.005630066,0.0352407,0.0010391924,0.000054186898],"about_ca_topic_score_codex":0.0024873447,"about_ca_topic_score_gemma":0.0011719095,"teacher_disagreement_score":0.0024873447,"about_ca_system_score_codex":0.00059798564,"about_ca_system_score_gemma":0.0002260295,"threshold_uncertainty_score":0.004945755},"labels":[],"label_agreement":null},{"id":"W2111410686","doi":"10.1086/383564","title":"A Comprehensive Study of the X‐Ray Bursts from the Magnetar Candidate 1E 2259+586","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":128,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Neutron star; Pulsar; Glitch; Gamma-ray burst; Power law; Astronomy; Statistics; Optics","score_opus":0.013322341138094312,"score_gpt":0.2962878204261556,"score_spread":0.28296547928806126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111410686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99852186,0.000097955315,0.00029380922,0.000022020187,0.0000019616648,0.000005226877,0.00039632898,0.000028359384,0.0006325469],"genre_scores_gemma":[0.99748385,0.00008322787,0.00048138216,0.000012900047,0.000010784994,0.0000054782704,0.0014570474,0.000017393113,0.00044776715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998671,0.0000134643,0.000012997384,0.00003548798,0.0000457648,0.000025151265],"domain_scores_gemma":[0.9994475,0.00011769115,0.00021706353,0.000054836637,0.00007649229,0.00008639891],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023022735,0.00021381721,0.00030441704,0.0015259876,0.00030345877,0.00043763072,0.00019482912,0.00013919552,0.0006585581],"category_scores_gemma":[0.00055937044,0.00010930411,0.00026463595,0.0009887349,0.00013927172,0.00020310505,0.00032709935,0.00018685327,0.0002843284],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026354368,0.00009136935,0.9147504,0.00006834326,0.00011174455,0.00088918593,0.00028880226,0.0014775975,0.058162645,0.00032647,0.0006198211,0.02295016],"study_design_scores_gemma":[0.000002076343,0.000052404386,0.9965912,0.000002501645,0.000011257859,0.00033516888,0.000050605347,0.0009754212,0.0011318997,0.000036808135,0.00080604374,0.0000046135942],"about_ca_topic_score_codex":0.00165597,"about_ca_topic_score_gemma":0.0029831666,"teacher_disagreement_score":0.00165597,"about_ca_system_score_codex":0.00017063085,"about_ca_system_score_gemma":0.00012730461,"threshold_uncertainty_score":0.0032927394},"labels":[],"label_agreement":null},{"id":"W2111437545","doi":"10.1086/588023","title":"Evidence for Nonhydrostatic Gas Motions in the Hot Interstellar Medium of Centaurus A","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Centaurus A; Interstellar medium; Physics; Astrophysics; Astronomy; Astrobiology; Galaxy; Radio galaxy","score_opus":0.048040057852140286,"score_gpt":0.2888038206666183,"score_spread":0.24076376281447803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111437545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966344,0.00089716504,0.00016101106,0.00008515832,0.00003386385,0.0000032779162,0.000097412114,0.000028000268,0.0020597654],"genre_scores_gemma":[0.9994784,0.00015922295,0.00006555281,0.000025960428,0.000035523208,0.000002320032,0.00007284011,0.0000033019364,0.00015687617],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999923,0.000009725613,0.0000057815564,0.000017195805,0.000015470743,0.000028697705],"domain_scores_gemma":[0.9994332,0.00014368932,0.00014695185,0.000056485525,0.000045499335,0.00017416646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014846202,0.00021649181,0.00024132298,0.0011858011,0.00063141825,0.0012703405,0.00042563234,0.0004891971,0.00204882],"category_scores_gemma":[0.0005889946,0.00027321532,0.00011029331,0.0004791574,0.0015532633,0.00085003424,0.0014881656,0.0003899987,0.00046691686],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008637583,0.0001441645,0.3013805,0.00029570452,0.0001395479,0.0018951033,0.0015952938,0.00076816714,0.6707912,0.0028559044,0.0007555246,0.018515062],"study_design_scores_gemma":[0.000033307682,0.00013854807,0.9865307,0.000014149824,0.000043163727,0.0005333825,0.00085865846,0.0006023927,0.00844538,0.0014036122,0.0013716416,0.000025140806],"about_ca_topic_score_codex":0.0016747501,"about_ca_topic_score_gemma":0.0014434727,"teacher_disagreement_score":0.00204882,"about_ca_system_score_codex":0.00024358212,"about_ca_system_score_gemma":0.00014900946,"threshold_uncertainty_score":0.0068539977},"labels":[],"label_agreement":null},{"id":"W2111482855","doi":"10.1088/0004-637x/790/1/60","title":"<i>NuSTAR</i>OBSERVATIONS OF X-RAY BURSTS FROM THE MAGNETAR 1E 1048.1–5937","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Black-body radiation; Astronomy; Spectral line; Flux (metallurgy); Cyclotron; Telescope; Pulsar; Electron; Radiation; Nuclear physics","score_opus":0.015849994655957298,"score_gpt":0.27931632896473374,"score_spread":0.2634663343087764,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111482855","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979893,0.00014318129,0.00025250993,0.000024280384,0.000007004017,0.0000046489763,0.00056650734,0.000048385682,0.00096421037],"genre_scores_gemma":[0.9960232,0.000104324594,0.0012903147,0.000022015814,0.00001953166,0.000005850592,0.002090591,0.000015954447,0.00042832817],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999095,0.000005728986,0.000008136973,0.0000275463,0.000029612564,0.00001954255],"domain_scores_gemma":[0.9997255,0.000020151978,0.00012924298,0.000031308165,0.000036314508,0.000057523936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001592734,0.00018710448,0.00023404475,0.0009991503,0.0003073534,0.00029874124,0.00024998575,0.0002313522,0.0006479516],"category_scores_gemma":[0.00030996944,0.00010299482,0.00015925609,0.0006845823,0.00014591502,0.00016466473,0.00032560155,0.00018959896,0.00028421945],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003939881,0.00011523753,0.83686846,0.00011220974,0.00012660507,0.0012312348,0.0004943158,0.00078575616,0.13200748,0.0002553323,0.0015797851,0.026029574],"study_design_scores_gemma":[0.000006378533,0.000095207106,0.9923161,0.000007852376,0.000028592654,0.0008466979,0.00006293424,0.00074790197,0.0040296125,0.0000537143,0.0017953044,0.000009624071],"about_ca_topic_score_codex":0.0024131886,"about_ca_topic_score_gemma":0.008549438,"teacher_disagreement_score":0.0024131886,"about_ca_system_score_codex":0.00022139528,"about_ca_system_score_gemma":0.00011141103,"threshold_uncertainty_score":0.0047983527},"labels":[],"label_agreement":null},{"id":"W2111515777","doi":"10.1088/0004-637x/767/1/33","title":"A MATHEMATICAL MODEL FOR AN HOURGLASS MAGNETIC FIELD","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Hourglass; Magnetic field; Cusp (singularity); Rotational symmetry; Coordinate system; Boundary value problem; Plane (geometry); Field (mathematics); Current (fluid)","score_opus":0.012302325311316432,"score_gpt":0.23891927127124712,"score_spread":0.2266169459599307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111515777","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08160613,0.0012653841,0.8151669,0.0028108237,0.0003210317,0.000081045764,0.00039597426,0.00039112184,0.097961545],"genre_scores_gemma":[0.8309112,0.0014241788,0.09340806,0.0005195644,0.0003622669,0.0003129444,0.00027666887,0.00019750543,0.07258759],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990344,0.00002278675,0.000004756266,0.000023975075,0.000026603115,0.000018481856],"domain_scores_gemma":[0.999801,0.000049419396,0.000050253293,0.000020126934,0.000046526235,0.000032688844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002714174,0.00033343068,0.00037545542,0.00057161576,0.0005144633,0.0012514734,0.0009348896,0.0010649166,0.0047971606],"category_scores_gemma":[0.00066177594,0.00020991192,0.00038983996,0.00040788096,0.0011884233,0.0014452677,0.0007072773,0.0005706493,0.0009111498],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000012158613,0.000013295476,0.00020206654,0.000055788663,0.000009242872,0.00021465588,0.00015045697,0.0775687,0.0042365473,0.9116971,0.0021318588,0.0037081128],"study_design_scores_gemma":[0.000030661617,0.000048431648,0.0005847367,0.000030556497,0.000010178154,0.00032755165,0.00013905978,0.6209041,0.00092378247,0.35271004,0.024262115,0.000028833383],"about_ca_topic_score_codex":0.002531812,"about_ca_topic_score_gemma":0.0015603446,"teacher_disagreement_score":0.0047971606,"about_ca_system_score_codex":0.000974871,"about_ca_system_score_gemma":0.0007664604,"threshold_uncertainty_score":0.016048074},"labels":[],"label_agreement":null},{"id":"W2111589745","doi":"10.3847/0004-637x/824/2/118","title":"THE KINETIC SUNYAEV–ZEL’DOVICH EFFECT FROM REIONIZATION: SIMULATED FULL-SKY MAPS AT ARCMINUTE RESOLUTION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Reionization; Physics; Cosmic microwave background; Sunyaev–Zel'dovich effect; Astrophysics; Redshift; Kinetic energy; Cosmic background radiation; Galaxy; Optics; Quantum mechanics","score_opus":0.0050791650737426934,"score_gpt":0.19882229143573968,"score_spread":0.19374312636199698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111589745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958664,0.00008402509,0.0019214901,0.00010560478,0.0000065526388,0.0000086763675,0.0005404384,0.00016924526,0.0012975998],"genre_scores_gemma":[0.99870014,0.000025838834,0.0006205515,0.00001245531,0.0000059292884,0.0000060590473,0.0004492573,0.00003270128,0.00014705384],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998779,0.00003491632,0.000004885017,0.00002162977,0.00001924678,0.000041490308],"domain_scores_gemma":[0.9990953,0.00044706638,0.00010951878,0.000103780425,0.00008455881,0.00015967594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041662433,0.000412649,0.00036487085,0.00043928335,0.00025182465,0.00060299487,0.0008349388,0.0005923598,0.001595151],"category_scores_gemma":[0.0015772306,0.0002663867,0.00063347793,0.00049099006,0.00044419718,0.00046764888,0.00064828986,0.0006202544,0.00013409753],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021453823,0.00007262016,0.027348742,0.00003237335,0.00010559251,0.0002002451,0.00007932966,0.9642454,0.0032015329,0.0019515541,0.0006426799,0.001905393],"study_design_scores_gemma":[0.000052121835,0.000027625523,0.019880036,0.0000056493955,0.00001735155,0.000040103427,0.00003338162,0.97806317,0.001005115,0.0005849715,0.0002762841,0.000014140733],"about_ca_topic_score_codex":0.011218629,"about_ca_topic_score_gemma":0.005496678,"teacher_disagreement_score":0.011218629,"about_ca_system_score_codex":0.0005889236,"about_ca_system_score_gemma":0.0002981022,"threshold_uncertainty_score":0.02230668},"labels":[],"label_agreement":null},{"id":"W2111779260","doi":"10.1088/0004-637x/726/1/41","title":"IDENTIFICATION OF H<sub>2</sub>CCC AS A DIFFUSE INTERSTELLAR BAND CARRIER","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Neon; Interstellar medium; Physics; Wavelength; Spectral line; Line (geometry); Absorption (acoustics); Atomic physics; Chemistry; Analytical Chemistry (journal); Astrophysics; Optics; Astronomy","score_opus":0.005211036862263336,"score_gpt":0.19917487754834828,"score_spread":0.19396384068608494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111779260","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99263,0.00026802206,0.0012216433,0.000052117204,0.00001873096,0.000008991619,0.0001856423,0.000038216844,0.0055767368],"genre_scores_gemma":[0.9962276,0.00011989346,0.0012442118,0.00006805054,0.000022700362,0.000012755504,0.00052073685,0.00001644121,0.0017675647],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993324,0.000002161914,0.0000015585335,0.000023999031,0.000019453848,0.000019621915],"domain_scores_gemma":[0.9998265,0.000020224328,0.000045477933,0.00002335522,0.000037512516,0.00004690303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000073784155,0.00016029175,0.000098274206,0.00040966467,0.000331314,0.00039450132,0.00030602506,0.000249161,0.0029118226],"category_scores_gemma":[0.00012240431,0.00010292796,0.00007505765,0.00037035887,0.00021405383,0.00023043595,0.00035972943,0.0003011611,0.00053447095],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036026663,0.00007591993,0.094472036,0.00008170187,0.000031117357,0.0003952037,0.00026083956,0.00025571274,0.8743292,0.0041335407,0.0014423616,0.024161937],"study_design_scores_gemma":[0.00006634627,0.0003822456,0.74551183,0.000047511232,0.00007898126,0.0012374901,0.00050231296,0.005452582,0.21962062,0.0014861498,0.02558432,0.000029746005],"about_ca_topic_score_codex":0.0026899292,"about_ca_topic_score_gemma":0.0051077525,"teacher_disagreement_score":0.0029118226,"about_ca_system_score_codex":0.00028691423,"about_ca_system_score_gemma":0.00013913633,"threshold_uncertainty_score":0.009741068},"labels":[],"label_agreement":null},{"id":"W2111881368","doi":"10.1086/338325","title":"Thermal Conduction in Clusters of Galaxies","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":456,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Thermal conduction; Physics; Thermal conductivity; Galaxy; Astrophysics; Galaxy cluster; Thermal; Chaotic; Plasma; Condensed matter physics; Wave vector; Meteorology; Nuclear physics; Quantum mechanics","score_opus":0.010031755980495336,"score_gpt":0.21735500994506146,"score_spread":0.20732325396456613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2111881368","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979809,0.00015791816,0.000959545,0.00002382403,0.000002250651,0.000002453037,0.000024382836,0.000026405047,0.0008224128],"genre_scores_gemma":[0.9996685,0.000026382962,0.00018315554,0.0000034047778,0.0000024581295,0.0000015959318,0.000022517035,0.000003124483,0.00008880861],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999088,0.000015443651,0.000002452192,0.000030485311,0.000011902387,0.000030833635],"domain_scores_gemma":[0.99937147,0.00015061,0.00018565424,0.00010192269,0.00008050708,0.00010989751],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002496223,0.00022926349,0.00020765093,0.0007969543,0.0003787899,0.00069974916,0.00030600667,0.00022949402,0.0005706634],"category_scores_gemma":[0.0017657225,0.00015814885,0.00016951708,0.0004406218,0.00062594353,0.00049141824,0.0005446235,0.00014747254,0.00012709998],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073312066,0.00004933399,0.7427958,0.000118783566,0.00019363691,0.00054677034,0.0023516556,0.14223549,0.052321665,0.03858263,0.0016664107,0.01840468],"study_design_scores_gemma":[0.0000624935,0.00013420105,0.61940986,0.000032636177,0.00010268044,0.0005608084,0.00054254034,0.33930525,0.010633417,0.02716156,0.0019846505,0.00006987242],"about_ca_topic_score_codex":0.0036728024,"about_ca_topic_score_gemma":0.0014356935,"teacher_disagreement_score":0.0036728024,"about_ca_system_score_codex":0.00049720495,"about_ca_system_score_gemma":0.00012535545,"threshold_uncertainty_score":0.0073028803},"labels":[],"label_agreement":null},{"id":"W2112240717","doi":"10.1088/0004-637x/790/2/101","title":"FAST RADIO BURST DISCOVERED IN THE ARECIBO PULSAR ALFA SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":519,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Canarie; Fonds Québécois de la Recherche sur la Nature et les Technologies; Universities Space Research Association; National Science Foundation","keywords":"Physics; Fast radio burst; Pulsar; Astrophysics; Astronomy; Radio telescope; Millisecond pulsar; Population; Interstellar medium; Galactic Center; Source counts; Green Bank Telescope; Galactic plane; Milky Way; Neutron star; Galaxy; Redshift","score_opus":0.016235157040772313,"score_gpt":0.3066251690854363,"score_spread":0.29039001204466397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112240717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966731,0.00026988558,0.00017761668,0.000070259644,0.000016714535,0.000007976581,0.00058571546,0.000024133427,0.0021745344],"genre_scores_gemma":[0.99652255,0.00036098962,0.0005045756,0.00007328838,0.000048052556,0.000014258979,0.0017402464,0.000008669317,0.0007272571],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998499,0.000016072052,0.0000071545733,0.000044892087,0.000034063753,0.000047847436],"domain_scores_gemma":[0.99956423,0.000039844555,0.0002053399,0.000042961205,0.000058832607,0.00008876429],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021428213,0.0002194567,0.00016853347,0.0015189984,0.00041976874,0.0005395974,0.00013428422,0.00028827396,0.00070044544],"category_scores_gemma":[0.0004523152,0.0001081938,0.00011037527,0.0010337401,0.00023325012,0.00019056391,0.00041599793,0.0002227247,0.00023486225],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018450813,0.00006108963,0.95380956,0.0000348957,0.00003847011,0.0005834433,0.0004637468,0.00004504909,0.021191733,0.0002489816,0.0017691029,0.021569425],"study_design_scores_gemma":[0.0000030537783,0.00001983815,0.99728394,0.0000034089685,0.0000059970644,0.00031745853,0.000091142676,0.000023540171,0.00025728837,0.000014061614,0.0019784747,0.0000017388357],"about_ca_topic_score_codex":0.0055788457,"about_ca_topic_score_gemma":0.009407536,"teacher_disagreement_score":0.0055788457,"about_ca_system_score_codex":0.00037400005,"about_ca_system_score_gemma":0.00016488975,"threshold_uncertainty_score":0.011092722},"labels":[],"label_agreement":null},{"id":"W2112285857","doi":"10.1086/587960","title":"A Transient Black Hole Low-Mass X-Ray Binary Candidate in Centaurus A","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Galaxy; Black hole (networking); Luminosity; Astronomy; Centaurus A; X-ray transient; Flux (metallurgy); X-ray binary; Stellar mass; Neutron star; Active galactic nucleus; Star formation","score_opus":0.011520333544467425,"score_gpt":0.2194431168732515,"score_spread":0.20792278332878406,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112285857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954833,0.00033228847,0.0002783476,0.000373985,0.0001250757,0.000015100203,0.00009234501,0.000039047118,0.003260495],"genre_scores_gemma":[0.99923885,0.000025737225,0.000066433255,0.00006353268,0.00005681465,0.0000023973644,0.00004723924,0.000006296709,0.00049277255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983346,0.000018238956,0.000016571306,0.00004129653,0.00002096388,0.000069450085],"domain_scores_gemma":[0.99923646,0.0001270061,0.00014168177,0.000087792774,0.000039716026,0.00036750067],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030979485,0.0005637452,0.0007636735,0.0017482152,0.0019046023,0.0025063392,0.0007986238,0.0021228145,0.0056087435],"category_scores_gemma":[0.0016038142,0.0002521307,0.00038774696,0.0006526358,0.0012378319,0.00071260525,0.0014235813,0.00068759,0.0014245578],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004623263,0.0010512158,0.5602025,0.00021857492,0.00015548064,0.32005194,0.0016503299,0.000735078,0.07497422,0.008907058,0.004689589,0.022740846],"study_design_scores_gemma":[0.00028893072,0.0020395627,0.66120297,0.00009819832,0.00020753047,0.30443764,0.0019371641,0.0034512677,0.012665989,0.008021687,0.0055365292,0.000112488444],"about_ca_topic_score_codex":0.00075910427,"about_ca_topic_score_gemma":0.0007190504,"teacher_disagreement_score":0.0056087435,"about_ca_system_score_codex":0.00048521505,"about_ca_system_score_gemma":0.00019465177,"threshold_uncertainty_score":0.018763125},"labels":[],"label_agreement":null},{"id":"W2112341914","doi":"10.1086/587133","title":"Kinemetry of SINS High‐Redshift Star‐Forming Galaxies: Distinguishing Rotating Disks from Major Mergers","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":268,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy; Kinematics; Velocity dispersion; Star formation; Accretion (finance); Galaxy merger; Astronomy; Luminous infrared galaxy; Galaxy formation and evolution; Classical mechanics","score_opus":0.010364378064179561,"score_gpt":0.21516096346125818,"score_spread":0.20479658539707862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112341914","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977963,0.0000641487,0.0008455314,0.000012074778,0.0000013329276,0.0000036975414,0.000066733926,0.0000176289,0.0011925424],"genre_scores_gemma":[0.9992893,0.000016639831,0.0005408567,0.000002950814,0.0000028690827,0.0000018892648,0.00009481853,0.0000018932237,0.000048850077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999813,0.00003975551,0.000024698038,0.000046208992,0.000042236505,0.000034116787],"domain_scores_gemma":[0.9983229,0.0003444363,0.0008321971,0.00018328163,0.00012249309,0.00019470786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039866945,0.00022404222,0.00026346833,0.0018109934,0.0004453462,0.0009460724,0.00020082388,0.00019791511,0.0011108953],"category_scores_gemma":[0.0020187574,0.00011204771,0.00012731638,0.0010682564,0.0006982493,0.0005191034,0.00051450817,0.00015515789,0.0002890969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000081677084,0.000023996558,0.9742485,0.00002003852,0.000015060548,0.00010980428,0.0007364199,0.000694625,0.010457998,0.0013819309,0.00010941689,0.012120486],"study_design_scores_gemma":[0.0000055462656,0.00004143956,0.995577,0.000003593795,0.00000888963,0.00024802162,0.00020397775,0.0016664547,0.0013282124,0.0004983206,0.00041285626,0.00000563503],"about_ca_topic_score_codex":0.0020511125,"about_ca_topic_score_gemma":0.0031967012,"teacher_disagreement_score":0.0020511125,"about_ca_system_score_codex":0.00033220815,"about_ca_system_score_gemma":0.00017568727,"threshold_uncertainty_score":0.0040783286},"labels":[],"label_agreement":null},{"id":"W2112356641","doi":"10.1088/0004-637x/739/1/52","title":"THE ATACAMA COSMOLOGY TELESCOPE: COSMOLOGICAL PARAMETERS FROM THE 2008 POWER SPECTRUM","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":403,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; CMB cold spot; Astrophysics; Sunyaev–Zel'dovich effect; South Pole Telescope; Cosmology; Cosmic background radiation; Spectral density; Dark energy; Observational cosmology; Astronomy; Redshift; Galaxy","score_opus":0.015191342557071259,"score_gpt":0.23069879124839965,"score_spread":0.2155074486913284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112356641","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6114375,0.002540105,0.048979245,0.004239532,0.00058633706,0.00025771436,0.14195788,0.0062177167,0.18378393],"genre_scores_gemma":[0.7909427,0.0010605517,0.064813375,0.00048810718,0.0003666377,0.00023604491,0.123287335,0.0027390218,0.016066292],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997856,0.00003513019,0.00000623347,0.000047896585,0.00009741176,0.000027762719],"domain_scores_gemma":[0.99907315,0.0001027645,0.00014335716,0.0001730684,0.00032380706,0.00018371418],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00084359915,0.00036902598,0.00029916278,0.0020895626,0.000673573,0.0013045726,0.00066213653,0.0005997228,0.007696106],"category_scores_gemma":[0.0030688376,0.00027528673,0.0003041351,0.0028348998,0.00023153558,0.0013930133,0.0009972873,0.00094884273,0.0029056934],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004679153,0.00022210578,0.2952311,0.00032162535,0.0003085878,0.0005323201,0.0027211974,0.012538761,0.008316426,0.036535513,0.40110672,0.24169779],"study_design_scores_gemma":[0.00014159075,0.000042777803,0.65590805,0.00010925019,0.00007294454,0.00048996427,0.00060015905,0.021091202,0.001814743,0.01968392,0.29991826,0.00012714634],"about_ca_topic_score_codex":0.03862235,"about_ca_topic_score_gemma":0.055002004,"teacher_disagreement_score":0.03862235,"about_ca_system_score_codex":0.00084027986,"about_ca_system_score_gemma":0.00077174173,"threshold_uncertainty_score":0.0767951},"labels":[],"label_agreement":null},{"id":"W2112561064","doi":"10.1086/512038","title":"Mid-Infrared Spectroscopy of High-Redshift Submillimeter Galaxies: First Results","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Galaxy; Redshift; Luminosity; Spectroscopy; Emission spectrum; Bolometer; Spitzer Space Telescope; Spectral line; Luminous infrared galaxy","score_opus":0.007279788189716737,"score_gpt":0.2169792883492743,"score_spread":0.20969950015955757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112561064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98876613,0.00206242,0.0027268566,0.00009975069,0.000010889331,0.000047765196,0.00077252206,0.00018148901,0.0053321514],"genre_scores_gemma":[0.9897697,0.0006563171,0.006668055,0.0001528477,0.000060963386,0.000023807945,0.0017188366,0.00003156387,0.00091785274],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99956864,0.00007332476,0.000018863619,0.000083102655,0.00013064947,0.00012545435],"domain_scores_gemma":[0.9990839,0.00020779962,0.00017049466,0.00015791293,0.00016068172,0.0002191363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011835035,0.00072849216,0.00035416867,0.0012101093,0.00053465157,0.0009108971,0.0006777356,0.0005419096,0.0011590879],"category_scores_gemma":[0.00059818686,0.00031426054,0.00049249583,0.00082597067,0.0003742891,0.0005663696,0.00075538154,0.00042320564,0.0004302389],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006399796,0.0009055946,0.8242811,0.00030359378,0.00033867997,0.000431798,0.0009924447,0.0010585941,0.11179369,0.0005748885,0.0015063975,0.05717332],"study_design_scores_gemma":[0.000012186826,0.00026320192,0.9863892,0.0000142912395,0.00008348597,0.00023691054,0.00012849219,0.0006545878,0.009716913,0.00014891403,0.0023376779,0.000014154934],"about_ca_topic_score_codex":0.0025846998,"about_ca_topic_score_gemma":0.004695202,"teacher_disagreement_score":0.0025846998,"about_ca_system_score_codex":0.0005140158,"about_ca_system_score_gemma":0.00012072744,"threshold_uncertainty_score":0.0062590837},"labels":[],"label_agreement":null},{"id":"W2112730149","doi":"10.1088/0004-637x/713/1/671","title":"SEARCHES FOR GRAVITATIONAL WAVES FROM KNOWN PULSARS WITH SCIENCE RUN 5 LIGO DATA","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; University of British Columbia","funders":"Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Govern de les Illes Balears; Fundacja na rzecz Nauki Polskiej; Scottish Funding Council; Commonwealth Scientific and Industrial Research Organisation; Scottish Universities Physics Alliance; Leverhulme Trust; Australian Government; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Pulsar; LIGO; Gravitational wave; Millisecond pulsar; Gravitational-wave observatory; Ephemeris; Amplitude; Binary pulsar; Crab Pulsar","score_opus":0.030127315411665995,"score_gpt":0.3508166741543607,"score_spread":0.32068935874269466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112730149","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99622935,0.000210377,0.0015803463,0.000037529462,0.0000060255256,0.000008473634,0.0007679956,0.00006579845,0.0010939873],"genre_scores_gemma":[0.99131864,0.00012128409,0.0025969474,0.00003851661,0.000018877074,0.000011444535,0.005435589,0.000012580347,0.00044604225],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993662,0.000073751195,0.000057807327,0.00013110111,0.00023554132,0.00013568363],"domain_scores_gemma":[0.9979621,0.0005061034,0.0007527794,0.00030980897,0.00015392424,0.0003151815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009328292,0.00028660588,0.00034798484,0.0020837162,0.0005286585,0.0009564834,0.00041294371,0.00039499806,0.0010751586],"category_scores_gemma":[0.0026084487,0.00021949563,0.0005014646,0.0012534782,0.00027284544,0.0005005584,0.00085540744,0.000380261,0.0002469975],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044870842,0.00009736212,0.9494345,0.00006539203,0.00026881776,0.00043276016,0.00041054795,0.0024371217,0.018464789,0.00086956273,0.00076405,0.026306365],"study_design_scores_gemma":[0.00005234806,0.00044358996,0.97573435,0.000019473558,0.0001856484,0.00064349646,0.00016300938,0.0069637382,0.008093977,0.0006497495,0.0070179068,0.000032632546],"about_ca_topic_score_codex":0.002879509,"about_ca_topic_score_gemma":0.0065736254,"teacher_disagreement_score":0.002879509,"about_ca_system_score_codex":0.0004002265,"about_ca_system_score_gemma":0.00047049418,"threshold_uncertainty_score":0.005725503},"labels":[],"label_agreement":null},{"id":"W2112754074","doi":"10.1088/0004-637x/767/1/10","title":"MAPPING<i>H</i>-BAND SCATTERED LIGHT EMISSION IN THE MYSTERIOUS SR21 TRANSITIONAL DISK","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Astronomical Observatory of Japan","keywords":"Radiative transfer; Circumstellar disk; Scattering; Opacity; Photosphere; Stars; Infrared; Polarization (electrochemistry); Near-infrared spectroscopy","score_opus":0.00801241118615688,"score_gpt":0.2141948584636324,"score_spread":0.2061824472774755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112754074","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982503,0.00006225818,0.00035760645,0.000023736355,0.0000019651752,0.000002236099,0.00005403753,0.000039156846,0.0012086547],"genre_scores_gemma":[0.9988765,0.000054455562,0.0007662753,0.000016322014,0.0000066903112,0.0000029763175,0.00009562947,0.000011108294,0.00016998604],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996305,0.0000019188549,0.0000016057268,0.000011921301,0.000009961369,0.000011572473],"domain_scores_gemma":[0.9998944,0.00001106678,0.000033252352,0.000018382372,0.000015740996,0.000027146149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000060532257,0.00016645633,0.00015076337,0.00025305935,0.00029755422,0.00042766938,0.00035895503,0.00025192767,0.0007811021],"category_scores_gemma":[0.00020272043,0.00013739183,0.0001549512,0.00015869114,0.00023672846,0.00024173263,0.0003462813,0.00027300627,0.0002815145],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003647654,0.0000584016,0.11501491,0.00010587273,0.000044048666,0.0011026722,0.0008749578,0.00087580853,0.8625488,0.0005882859,0.00039325817,0.018028237],"study_design_scores_gemma":[0.00003255902,0.00031930723,0.9354202,0.000025849025,0.000067511486,0.0016580527,0.0008662635,0.0046568247,0.05272441,0.00047834803,0.0037256074,0.00002518828],"about_ca_topic_score_codex":0.0009138859,"about_ca_topic_score_gemma":0.0015015756,"teacher_disagreement_score":0.0009138859,"about_ca_system_score_codex":0.00017857394,"about_ca_system_score_gemma":0.00009126874,"threshold_uncertainty_score":0.002613008},"labels":[],"label_agreement":null},{"id":"W2112888571","doi":"10.1088/0004-637x/805/1/85","title":"ERRATUM: “TIMING OF FIVE MILLISECOND PULSARS DISCOVERED IN THE PALFA SURVEY” (2015, ApJ, 800, 123)","year":2015,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Tropical and Extratropical Cyclones Research","field":"Earth and Planetary Sciences","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Library science; Astronomy; Astrophysics","score_opus":0.038466478275004976,"score_gpt":0.2779009482075804,"score_spread":0.2394344699325754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112888571","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.015161802,0.005617432,0.0029523745,0.052386254,0.8683001,0.00010610728,0.026456637,0.0019382845,0.027081037],"genre_scores_gemma":[0.16036077,0.019517263,0.02127107,0.05457639,0.19741875,0.0004880358,0.11417589,0.0029425758,0.42924926],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99939024,0.000058304468,0.00015755348,0.00013168594,0.00020056819,0.00006161111],"domain_scores_gemma":[0.9951609,0.0005934824,0.0006126369,0.0004303666,0.002939812,0.00026285686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008125161,0.001127956,0.00049618323,0.0038228051,0.0017698633,0.0014580236,0.0011909078,0.0014890848,0.024573207],"category_scores_gemma":[0.009330367,0.00052848744,0.00050636724,0.002612116,0.0006681943,0.0012981021,0.0009827961,0.0019541858,0.016254814],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000066994995,0.000016605545,0.0039405064,0.00013926279,0.000018227365,0.00028785501,0.00006162229,0.000094169634,0.0002711629,0.00075592776,0.9771721,0.017175598],"study_design_scores_gemma":[0.000037651123,0.0000809841,0.03538856,0.00029735974,0.000040323433,0.00066824956,0.00023498407,0.00028421657,0.00060205354,0.0006531108,0.9616671,0.00004529321],"about_ca_topic_score_codex":0.02308478,"about_ca_topic_score_gemma":0.02064796,"teacher_disagreement_score":0.024573207,"about_ca_system_score_codex":0.0012656474,"about_ca_system_score_gemma":0.0016892047,"threshold_uncertainty_score":0.08220559},"labels":[],"label_agreement":null},{"id":"W2112908490","doi":"10.1088/0004-637x/790/1/13","title":"LINEAR STABILITY OF MAGNETIZED MASSIVE PROTOPLANETARY DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Polytropic process; Accretion (finance); Instability; Angular momentum; Protoplanetary disk; Astrophysics; Magnetic field; Scale height; Rotational symmetry; Angular velocity; Turbulence; Axial symmetry; Gravitation; Mechanics; Classical mechanics; Stars; Quantum mechanics","score_opus":0.011052136052204599,"score_gpt":0.23329594370962906,"score_spread":0.22224380765742446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112908490","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98753136,0.0002600074,0.0074801734,0.00011994088,0.0000072279745,0.000009380941,0.00003672167,0.00010062779,0.0044546532],"genre_scores_gemma":[0.99871504,0.000054568187,0.0005267128,0.0000107519,0.0000042935203,0.0000066529733,0.000023157134,0.0000057772495,0.0006529677],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999534,0.000007780186,0.0000020666582,0.000011737483,0.000015032528,0.000010071612],"domain_scores_gemma":[0.9998499,0.000031516684,0.00005341367,0.000010624487,0.000030220053,0.000024273188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000978187,0.00022305048,0.00019942618,0.0002833504,0.0003300278,0.00068467134,0.00037461627,0.00024919,0.0005770939],"category_scores_gemma":[0.0005370777,0.00012571551,0.00016346533,0.00012795631,0.0006907949,0.0003349022,0.0005854272,0.00020960173,0.00016046608],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005748862,0.00008468598,0.018674951,0.0001488691,0.00006905819,0.0007755825,0.0005690348,0.7363599,0.19296655,0.036168847,0.0007409816,0.012866788],"study_design_scores_gemma":[0.0000434633,0.000109993656,0.006193243,0.000010939763,0.000008644991,0.00009965846,0.00013679093,0.97820616,0.0067432714,0.008094136,0.0003334992,0.000020212927],"about_ca_topic_score_codex":0.002331475,"about_ca_topic_score_gemma":0.0008549499,"teacher_disagreement_score":0.002331475,"about_ca_system_score_codex":0.0006852438,"about_ca_system_score_gemma":0.00027172602,"threshold_uncertainty_score":0.0049718022},"labels":[],"label_agreement":null},{"id":"W2112945935","doi":"10.1086/511413","title":"Spectroscopy of Globular Clusters out to Large Radius in the Sombrero Galaxy","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Velocity dispersion; Galaxy; Galaxy rotation curve; RADIUS; Astronomy; Galaxy cluster; Star cluster; Galaxy formation and evolution","score_opus":0.009883871421548689,"score_gpt":0.253553286144229,"score_spread":0.2436694147226803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2112945935","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956554,0.00016079262,0.00045067375,0.00005621773,0.00000851714,0.0000069267294,0.00062348385,0.00010609728,0.002931744],"genre_scores_gemma":[0.99508876,0.0001352572,0.0016928989,0.00006044468,0.000021983353,0.0000091276015,0.0019008705,0.00002702256,0.001063615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997539,0.000012747393,0.000009240969,0.000079272104,0.00006974235,0.00007512485],"domain_scores_gemma":[0.999622,0.000028617993,0.00010105334,0.00006194162,0.00006347381,0.00012288513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028474318,0.00024031111,0.00021322945,0.0017442054,0.0005089826,0.0005308419,0.00042730971,0.00032664623,0.0014582576],"category_scores_gemma":[0.0004890712,0.00024989853,0.00027567966,0.0008782533,0.00019855113,0.00027566336,0.0007573593,0.00027816088,0.00046628702],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030210335,0.00010805369,0.88596004,0.00007281252,0.00012175178,0.00033547133,0.0009360149,0.001158907,0.08061902,0.00046612817,0.0025697746,0.02734981],"study_design_scores_gemma":[0.000014463632,0.00005363897,0.9933514,0.000013316875,0.00002286798,0.00013150294,0.00019506083,0.0013649823,0.0020137175,0.000097977856,0.0027291605,0.00001195191],"about_ca_topic_score_codex":0.015407383,"about_ca_topic_score_gemma":0.039310466,"teacher_disagreement_score":0.015407383,"about_ca_system_score_codex":0.0007770519,"about_ca_system_score_gemma":0.00018783359,"threshold_uncertainty_score":0.030635417},"labels":[],"label_agreement":null},{"id":"W2113035541","doi":"10.1086/509318","title":"The Signature of Primordial Grain Growth in the Polarized Light of the AU Microscopii Debris Disk","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Debris disk; Physics; Polarization (electrochemistry); Linear polarization; Cosmic dust; Astrophysics; Sublimation (psychology); Scattering; Silicate; Porosity; Optics; Materials science; Stars; Planetary system; Astronomy; Laser; Composite material; Chemistry","score_opus":0.002574148475549091,"score_gpt":0.18710431686153456,"score_spread":0.18453016838598546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113035541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977362,0.0000851924,0.000549345,0.000022211096,0.000003126487,0.0000032024552,0.00014494383,0.000025815963,0.0014299564],"genre_scores_gemma":[0.9988292,0.00003902178,0.0006525683,0.000010217157,0.000004231553,0.0000030497572,0.00020264315,0.000009233497,0.00024985697],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999577,0.0000029702617,0.0000010973401,0.000012224115,0.000009692063,0.000016423952],"domain_scores_gemma":[0.9998215,0.00003583673,0.000028800234,0.0000255395,0.000052316766,0.00003605221],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000067186425,0.00010924263,0.00008239173,0.00042790567,0.0002920339,0.00045322505,0.00016968203,0.0001697199,0.00065857347],"category_scores_gemma":[0.00022662616,0.0001614631,0.00008483693,0.0002625285,0.00019786415,0.00015768701,0.00019354303,0.00020496488,0.00016069699],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041192034,0.0000670845,0.3433843,0.00004965951,0.000033830176,0.00091977173,0.00060366146,0.0010514077,0.63729674,0.000776965,0.00053813815,0.014866587],"study_design_scores_gemma":[0.000012421756,0.00005738221,0.95268047,0.0000067677443,0.000011084791,0.00037791426,0.00014120714,0.0025905676,0.041908473,0.00016918698,0.002035268,0.000009341909],"about_ca_topic_score_codex":0.0020470833,"about_ca_topic_score_gemma":0.0022561506,"teacher_disagreement_score":0.0020470833,"about_ca_system_score_codex":0.00027381748,"about_ca_system_score_gemma":0.000087032815,"threshold_uncertainty_score":0.004070282},"labels":[],"label_agreement":null},{"id":"W2113058576","doi":"10.1088/0004-637x/787/1/34","title":"POWER SPECTRUM ANALYSIS OF POLARIZED EMISSION FROM THE CANADIAN GALACTIC PLANE SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"National Research Council Canada; University of Alberta; Dominion Astrophysical Observatory; Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Astronomy; Spectral index; Observatory; Telescope; Supernova; Spectral line; Galaxy","score_opus":0.007530258111756007,"score_gpt":0.21145056454733607,"score_spread":0.20392030643558007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113058576","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8719311,0.0006383105,0.0054909247,0.00033838916,0.000039036684,0.00011803797,0.08477511,0.00043506082,0.03623395],"genre_scores_gemma":[0.90662307,0.0006996134,0.004957493,0.00007904757,0.00002157089,0.000063125015,0.08201442,0.00017010694,0.00537145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994703,0.000026810374,0.000010400394,0.000085221065,0.00026154306,0.00014578279],"domain_scores_gemma":[0.9989039,0.00006911936,0.00010151393,0.000069413574,0.0007573224,0.00009882929],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037637464,0.000382507,0.00023268795,0.004075571,0.00068174454,0.0010063363,0.0005490449,0.00015192563,0.0035864862],"category_scores_gemma":[0.0016318875,0.00015377882,0.00035614395,0.0066387854,0.0003164152,0.00021582303,0.00039251373,0.00028778324,0.0006685969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023455327,0.000048688915,0.84672636,0.00018221753,0.0004180596,0.0003731525,0.0008209879,0.011282434,0.009022393,0.005043721,0.04687396,0.07897348],"study_design_scores_gemma":[0.0000049753894,0.000005689084,0.97309846,0.000017108865,0.00002607905,0.00007451553,0.00032558187,0.004043677,0.0007167882,0.00018043966,0.021486808,0.000019798934],"about_ca_topic_score_codex":0.9136837,"about_ca_topic_score_gemma":0.92528564,"teacher_disagreement_score":0.08631629,"about_ca_system_score_codex":0.0054291957,"about_ca_system_score_gemma":0.004462468,"threshold_uncertainty_score":0.17364919},"labels":[],"label_agreement":null},{"id":"W2113093682","doi":"10.1088/0004-637x/775/1/20","title":"THE RICH GLOBULAR CLUSTER SYSTEM OF ABELL 1689 AND THE RADIAL DEPENDENCE OF THE GLOBULAR CLUSTER FORMATION EFFICIENCY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Galaxy cluster; Virial mass; Galaxy; Abell 2744; Cluster (spacecraft); Milky Way; Galaxy groups and clusters; Population","score_opus":0.0035244934134061527,"score_gpt":0.1818394110463725,"score_spread":0.17831491763296634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113093682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99809545,0.000055854314,0.000048400707,0.000027962482,0.0000013159173,0.0000015817338,0.00017836668,0.0000051088996,0.001585902],"genre_scores_gemma":[0.999292,0.00001689705,0.000033507215,0.000004814437,0.0000017763898,9.3369687e-7,0.00024196393,0.0000032099829,0.00040490236],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999285,0.000009203934,0.0000031899438,0.000022109092,0.000012033742,0.000024996705],"domain_scores_gemma":[0.9994406,0.00009237893,0.00018769305,0.000043539483,0.000073916606,0.000161921],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019194068,0.00009650721,0.00013442451,0.0005714981,0.00038359722,0.0004490902,0.00017020949,0.00016703013,0.002040567],"category_scores_gemma":[0.0008280066,0.00008883534,0.000081974336,0.0003995251,0.00022814704,0.00022727056,0.00043078515,0.00013642902,0.00037056688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005800183,0.00009658199,0.9433408,0.000027414264,0.000072027,0.00033305283,0.00035143175,0.0032445432,0.038349655,0.003394862,0.001560659,0.008648942],"study_design_scores_gemma":[0.0000041602007,0.000014374438,0.9973273,0.0000018219708,0.00000703339,0.000058465066,0.000081941325,0.0013656693,0.00044945662,0.00024145805,0.00044358463,0.0000047325616],"about_ca_topic_score_codex":0.024244368,"about_ca_topic_score_gemma":0.03128686,"teacher_disagreement_score":0.024244368,"about_ca_system_score_codex":0.00066315045,"about_ca_system_score_gemma":0.00022092358,"threshold_uncertainty_score":0.04820651},"labels":[],"label_agreement":null},{"id":"W2113244389","doi":"10.1088/0004-637x/767/2/116","title":"JOINT ANALYSIS OF CLUSTER OBSERVATIONS. II. CHANDRA/XMM-NEWTON X-RAY AND WEAK LENSING SCALING RELATIONS FOR A SAMPLE OF 50 RICH CLUSTERS OF GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":241,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Scaling; Weak gravitational lensing; Galaxy cluster; Bimodality; Centroid; Population; Line-of-sight; Galaxy; Cluster (spacecraft)","score_opus":0.018311354875546457,"score_gpt":0.22076574789949466,"score_spread":0.2024543930239482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113244389","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986236,0.00013748041,0.0002731104,0.000012962985,0.000001872051,0.000004653595,0.0006848308,0.00002161999,0.00023991123],"genre_scores_gemma":[0.9980204,0.000040678544,0.00037220985,0.0000054345132,0.0000049815944,0.000005545167,0.0013827144,0.000010772873,0.0001572066],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99931633,0.0001214396,0.00006354366,0.00024111843,0.00014164175,0.000115979536],"domain_scores_gemma":[0.99686027,0.0007370911,0.00085977383,0.0007156095,0.0004427699,0.00038449335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010731483,0.00030673982,0.00031928395,0.0020502917,0.00042918656,0.0007817794,0.00026105042,0.0001736461,0.0009840496],"category_scores_gemma":[0.0033836174,0.00017746689,0.0004790243,0.0015585924,0.00027540038,0.00033460796,0.00081723987,0.00022520903,0.00035551333],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011898874,0.000010776368,0.991469,0.000014017605,0.00017205575,0.000038102822,0.00010527772,0.0005607125,0.002903668,0.00008554465,0.00020725759,0.004314526],"study_design_scores_gemma":[0.0000018559437,0.00001696733,0.99837023,0.0000015774972,0.0000308128,0.000046065543,0.000048434445,0.00095535803,0.00029958284,0.000031393272,0.00019393206,0.0000038053793],"about_ca_topic_score_codex":0.0110317385,"about_ca_topic_score_gemma":0.0114634195,"teacher_disagreement_score":0.0110317385,"about_ca_system_score_codex":0.00033792757,"about_ca_system_score_gemma":0.00025182607,"threshold_uncertainty_score":0.021935046},"labels":[],"label_agreement":null},{"id":"W2113364565","doi":"10.1086/525524","title":"Low-Mass X-Ray Binaries and Globular Clusters in Centaurus A","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Astrophysics; Physics; Low Mass; Hubble space telescope; Observatory; X-ray; Astronomy; Population; Galaxy; Stars; Medicine","score_opus":0.007530758228624171,"score_gpt":0.2233956730448756,"score_spread":0.21586491481625142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113364565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984688,0.00055839366,0.000050615225,0.00012988265,0.000012060582,0.0000014986557,0.00009384388,0.000008264592,0.0006765097],"genre_scores_gemma":[0.9995067,0.00007413972,0.000014320293,0.000016486643,0.00002119341,8.95073e-7,0.00010788912,0.0000023193677,0.0002559537],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985456,0.000028991002,0.000012969659,0.000036972888,0.000016472513,0.00004996276],"domain_scores_gemma":[0.99831414,0.00038945497,0.00048924336,0.00008622385,0.00008093858,0.000640058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047708084,0.0002605141,0.0004937624,0.0024519302,0.0013672366,0.00235414,0.0005712789,0.0007439712,0.005363998],"category_scores_gemma":[0.0018930564,0.00021304553,0.00018888117,0.0023122535,0.0014936777,0.00070746196,0.0016146156,0.00061171275,0.00065149355],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035910125,0.00007434981,0.99126995,0.000020850755,0.000055526605,0.0003180466,0.00035745677,0.0003055522,0.001079911,0.0013236544,0.00071225304,0.004123291],"study_design_scores_gemma":[0.000011930988,0.000027138789,0.9975491,0.00000912696,0.000021702852,0.00017044962,0.00037981328,0.00038243385,0.00007365432,0.0011673451,0.00019954641,0.0000077544655],"about_ca_topic_score_codex":0.015281615,"about_ca_topic_score_gemma":0.01287562,"teacher_disagreement_score":0.015281615,"about_ca_system_score_codex":0.00073826284,"about_ca_system_score_gemma":0.00031412367,"threshold_uncertainty_score":0.030385315},"labels":[],"label_agreement":null},{"id":"W2113426348","doi":"10.1086/421771","title":"Photometric Variability among the Brightest Asymptotic Giant Branch Stars near the Center of M32","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Asymptotic giant branch; Stars; Galactic Center; Amplitude; Population; Giant star; Virgo Cluster; Stellar population; Star cluster","score_opus":0.0074882448999477646,"score_gpt":0.20998161532582554,"score_spread":0.20249337042587778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113426348","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997179,0.000017212638,0.00003837274,0.0000035548987,2.9661288e-7,7.829643e-7,0.000036915164,0.0000043753366,0.0001805429],"genre_scores_gemma":[0.9994443,0.000017592649,0.00019705661,0.0000035102576,0.0000017615724,0.0000019941042,0.00017502392,0.0000031197249,0.00015554513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993455,0.000007763778,0.000004358658,0.00002169359,0.000013110981,0.000018476898],"domain_scores_gemma":[0.99967587,0.0000328093,0.00010304983,0.000046461137,0.00004093808,0.00010083564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017463406,0.0001703241,0.00025431032,0.0010697172,0.0003748537,0.0002660255,0.00015889388,0.00019253383,0.00097376877],"category_scores_gemma":[0.0006318959,0.00012738025,0.00013412336,0.0006385898,0.00028236932,0.00026802425,0.0006663196,0.00016731769,0.0003091838],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040261683,0.000036399335,0.88097215,0.000024087694,0.000026728943,0.00026173805,0.0012488097,0.00021231109,0.10381029,0.000117796946,0.00023503297,0.012652046],"study_design_scores_gemma":[0.0000031960842,0.000035688903,0.99868804,0.0000015607577,0.0000034446102,0.00019564044,0.000098645054,0.00011123109,0.00067129347,0.00002732149,0.0001619445,0.0000020287434],"about_ca_topic_score_codex":0.0024015172,"about_ca_topic_score_gemma":0.0061948593,"teacher_disagreement_score":0.0024015172,"about_ca_system_score_codex":0.0002515741,"about_ca_system_score_gemma":0.00009858893,"threshold_uncertainty_score":0.004775107},"labels":[],"label_agreement":null},{"id":"W2113553616","doi":"10.1086/319776","title":"An Exploration of the Paradigm for the 2–3 Hour Period Gap in Cataclysmic Variables","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":286,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Bishop's University","funders":"","keywords":"Cataclysmic variable star; Period (music); Stellar evolution; Current (fluid); Variable star; Binary star","score_opus":0.03846767194571557,"score_gpt":0.27033636032693503,"score_spread":0.23186868838121946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113553616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89782095,0.0048275026,0.058472466,0.009913926,0.00029909442,0.000040553794,0.0002317997,0.00014312848,0.02825054],"genre_scores_gemma":[0.9940164,0.00053470186,0.004200443,0.00028675498,0.00012152986,0.000028961915,0.000052674324,0.00003331043,0.0007250647],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.9997851,0.000052720647,0.000010463411,0.00007998843,0.000040314717,0.00003146404],"domain_scores_gemma":[0.9990777,0.00039707278,0.00022126472,0.0001407813,0.000075394186,0.000087768945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011062467,0.00021760499,0.00036856768,0.0005346536,0.00076679897,0.002194403,0.0009598502,0.0009253024,0.0027707587],"category_scores_gemma":[0.0029352964,0.0001653777,0.00034421583,0.0005311506,0.0021981543,0.0038890662,0.0013906844,0.0016597023,0.0002135613],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029610354,0.00007487077,0.045777123,0.00013970608,0.000026391468,0.00047359598,0.001905044,0.0040310095,0.010312084,0.8978943,0.0018117153,0.03725808],"study_design_scores_gemma":[0.00006698267,0.00022849739,0.04831453,0.00007771178,0.000025057301,0.0011659808,0.0022167943,0.034046493,0.0019148756,0.8897831,0.022106461,0.00005352306],"about_ca_topic_score_codex":0.0005307495,"about_ca_topic_score_gemma":0.0004392402,"teacher_disagreement_score":0.0027707587,"about_ca_system_score_codex":0.0008298137,"about_ca_system_score_gemma":0.00052578154,"threshold_uncertainty_score":0.009269059},"labels":[],"label_agreement":null},{"id":"W2113596630","doi":"10.1086/342120","title":"Constraints on Ω<sub><i>m</i></sub>and σ<sub>8</sub>from Weak Lensing in Red‐Sequence Cluster Survey Fields","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":183,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Prior probability; Redshift; Galaxy; Astrophysics; Weak gravitational lensing; Gravitational lens; Galaxy cluster; Gaussian; Cosmic background radiation; Observational cosmology; Statistics; Mathematics; Optics; Bayesian probability; Quantum mechanics","score_opus":0.01839470696698998,"score_gpt":0.21502195703726126,"score_spread":0.1966272500702713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113596630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9918337,0.00028968143,0.0046334183,0.00014586949,0.0000064970727,0.0000073699175,0.000993756,0.00011800047,0.0019717133],"genre_scores_gemma":[0.995329,0.00013890477,0.0028314232,0.000079544865,0.00002960738,0.000012215621,0.001320243,0.000052386255,0.00020658318],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99833715,0.00042680124,0.0001684635,0.00041063258,0.00040409056,0.00025286496],"domain_scores_gemma":[0.9829967,0.008892104,0.003325525,0.0023015079,0.0012198843,0.0012643158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0041026557,0.001056657,0.0008198239,0.0018289152,0.00055247,0.0018981212,0.0010166875,0.00071201095,0.0022420199],"category_scores_gemma":[0.017186306,0.0010026891,0.0007174802,0.0014580056,0.0009478091,0.0009677058,0.001231061,0.0007724241,0.0007872288],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003599201,0.000042725856,0.9349326,0.0001300677,0.0002712656,0.00022471837,0.0002930433,0.022711039,0.020537134,0.0034603572,0.00092702353,0.016110137],"study_design_scores_gemma":[0.000046588604,0.000059495065,0.9683583,0.000058397094,0.00014167272,0.00009895275,0.00015907893,0.020846387,0.0043824315,0.0040903897,0.0016942676,0.00006403624],"about_ca_topic_score_codex":0.015790354,"about_ca_topic_score_gemma":0.023742676,"teacher_disagreement_score":0.015790354,"about_ca_system_score_codex":0.0010547347,"about_ca_system_score_gemma":0.0010287013,"threshold_uncertainty_score":0.031396866},"labels":[],"label_agreement":null},{"id":"W2113799640","doi":"10.1088/0004-637x/788/2/120","title":"IMAGING THE SUPERMASSIVE BLACK HOLE SHADOW AND JET BASE OF M87 WITH THE EVENT HORIZON TELESCOPE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Supermassive black hole; Schwarzschild radius; Very-long-baseline interferometry; Black hole (networking); Superluminal motion; Event horizon; Jet (fluid); Sagittarius A*; Galaxy","score_opus":0.0042195525680001735,"score_gpt":0.19815837869141212,"score_spread":0.19393882612341196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113799640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932146,0.00008148,0.003173366,0.00009466804,0.0000079223755,0.000018069295,0.00029838958,0.00014724942,0.0029642137],"genre_scores_gemma":[0.9948159,0.000044325487,0.0043044146,0.000028154178,0.0000064849346,0.0000061267515,0.00044328975,0.00004208701,0.00030916496],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998989,0.000017982109,0.000002262257,0.0000146452085,0.00003119431,0.00003490174],"domain_scores_gemma":[0.9998098,0.000044544133,0.00003510197,0.00003130155,0.000026191314,0.000052941527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027074647,0.00031501285,0.00030743692,0.00031981315,0.00025043805,0.00052638876,0.00044227077,0.00034783373,0.00081576075],"category_scores_gemma":[0.00045941604,0.00021737938,0.00049408845,0.00029800137,0.00024758978,0.0003152998,0.00046833744,0.00036847108,0.00019727772],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013701735,0.0008331341,0.18484765,0.00019279987,0.00044059573,0.0028862604,0.0016243841,0.533692,0.22268271,0.009138615,0.005851512,0.036440164],"study_design_scores_gemma":[0.00016156447,0.00041562514,0.2488516,0.000024871197,0.00007952508,0.00032456877,0.00038483352,0.72948915,0.016021645,0.0016137114,0.0025892071,0.00004373794],"about_ca_topic_score_codex":0.009751176,"about_ca_topic_score_gemma":0.01173493,"teacher_disagreement_score":0.009751176,"about_ca_system_score_codex":0.00078240957,"about_ca_system_score_gemma":0.00033132598,"threshold_uncertainty_score":0.019388855},"labels":[],"label_agreement":null},{"id":"W2113891486","doi":"10.1086/367831","title":"An X‐Ray Investigation of the NGC 346 Field in the Small Magellanic Cloud. II. The Field Population","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astrophysics; Physics; Small Magellanic Cloud; Luminosity; Sky; Telescope; Population; Cluster (spacecraft); X-ray; Field of view; Field (mathematics); Luminosity function; Astronomy; Point source; Absorption (acoustics); Galaxy; Optics","score_opus":0.012507452707959625,"score_gpt":0.22699400929950025,"score_spread":0.21448655659154062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2113891486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988734,0.00011132762,0.000072199626,0.000022282476,0.0000016736929,0.0000069236953,0.00021635249,0.0000050563035,0.00069072866],"genre_scores_gemma":[0.9974039,0.0001391905,0.00031658332,0.000015733493,0.000016366857,0.0000052257624,0.0009201233,0.0000043163573,0.0011785757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999889,0.000014094554,0.0000039803544,0.00003254955,0.00002114899,0.00003930755],"domain_scores_gemma":[0.9997409,0.000021171081,0.000056278604,0.00002559198,0.000045701414,0.00011038662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021103874,0.0002308463,0.00013700826,0.0014749665,0.00071396335,0.00027590262,0.0002066576,0.00015046178,0.0021345438],"category_scores_gemma":[0.00025001244,0.00008164053,0.0001231078,0.00092070043,0.00022464542,0.00029156456,0.00035344332,0.00015710441,0.0006229939],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004337265,0.00032602987,0.9368463,0.0000379811,0.000020902986,0.00061761215,0.0011112116,0.00019133287,0.02573394,0.0009261342,0.0017276446,0.03202719],"study_design_scores_gemma":[0.000006585773,0.000107050226,0.99625385,0.0000026124917,0.0000055958653,0.000480254,0.00023424994,0.00021624225,0.0003991347,0.00008027101,0.0022122045,0.0000019834797],"about_ca_topic_score_codex":0.009474233,"about_ca_topic_score_gemma":0.013516213,"teacher_disagreement_score":0.009474233,"about_ca_system_score_codex":0.0003580166,"about_ca_system_score_gemma":0.00018183893,"threshold_uncertainty_score":0.018838167},"labels":[],"label_agreement":null},{"id":"W2114042356","doi":"10.1086/510280","title":"Collisional Particle Disks","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Particle (ecology); Geology","score_opus":0.009725087065692334,"score_gpt":0.23676628839498615,"score_spread":0.2270412013292938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114042356","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08915713,0.00018330493,0.89918643,0.00013088125,0.00011078454,0.00010665826,0.00015574819,0.00087059167,0.010098462],"genre_scores_gemma":[0.4905721,0.00014720834,0.5009105,0.000121254954,0.00003548682,0.00021462966,0.00031231294,0.00038622826,0.0073003424],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983275,0.000022503946,0.000009104512,0.00003456245,0.00007862563,0.000022431823],"domain_scores_gemma":[0.99963427,0.00010621269,0.00003884878,0.00009093607,0.000088986744,0.000040676572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003955501,0.00032365858,0.0004151919,0.00031491616,0.000698697,0.0008348846,0.0020941163,0.0007358361,0.0031255572],"category_scores_gemma":[0.0016284976,0.00037221092,0.0004338198,0.0003007729,0.00048403358,0.000934584,0.0010628682,0.0005501452,0.0006892597],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015347867,0.00009936109,0.005582893,0.00009247412,0.00010462474,0.00037817174,0.00033755007,0.82993823,0.016053855,0.058398563,0.0025175111,0.08634325],"study_design_scores_gemma":[0.000023548126,0.000015216925,0.00023732602,0.0000032590497,0.00000530754,0.000065429485,0.000012553372,0.9920243,0.0016192473,0.0032149598,0.0027705384,0.000008280561],"about_ca_topic_score_codex":0.0033645653,"about_ca_topic_score_gemma":0.0033772402,"teacher_disagreement_score":0.0033645653,"about_ca_system_score_codex":0.00054571935,"about_ca_system_score_gemma":0.00078625156,"threshold_uncertainty_score":0.010456026},"labels":[],"label_agreement":null},{"id":"W2114086484","doi":"10.1088/0004-637x/770/2/142","title":"THE ABUNDANCE OF H<sub>2</sub>O AND HDO IN ORION KL FROM<i>HERSCHEL</i>/HIFI","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Spectral line; Abundance (ecology); Molecular absorption; Plateau (mathematics); Ridge; Absorption spectroscopy; Abundance of the chemical elements; Molecular cloud","score_opus":0.005961440887906592,"score_gpt":0.2063209892886667,"score_spread":0.20035954840076012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114086484","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907863,0.000029398521,0.000057144265,0.0000066638613,7.907635e-7,0.0000020339392,0.00046559266,0.000012503239,0.00034713556],"genre_scores_gemma":[0.9972156,0.000029784884,0.00034853554,0.000019561125,0.0000045374895,0.0000044865214,0.002097768,0.000013611931,0.00026615345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988735,0.0000066499924,0.0000055227515,0.0000476815,0.00002572472,0.000027115555],"domain_scores_gemma":[0.99977726,0.000019212988,0.00010613826,0.000018253539,0.000025071296,0.000054036893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013423916,0.00021700663,0.00012758058,0.00092999265,0.0002394628,0.00041557042,0.0002939255,0.00021595723,0.0008631932],"category_scores_gemma":[0.00023116943,0.00015900057,0.0001532216,0.000462795,0.00023379186,0.00026839916,0.0003475316,0.00015815547,0.00022874713],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012695149,0.000040518597,0.9569087,0.000020263036,0.000045475197,0.00012796074,0.00021155366,0.000539647,0.036332183,0.000070510854,0.00032700936,0.005249157],"study_design_scores_gemma":[0.0000026599523,0.000010655823,0.99825794,0.0000013831311,0.000007712875,0.00004012811,0.000035195335,0.00045199873,0.0008398545,0.000017170347,0.00033297256,0.0000023021878],"about_ca_topic_score_codex":0.009291042,"about_ca_topic_score_gemma":0.01590328,"teacher_disagreement_score":0.009291042,"about_ca_system_score_codex":0.00052192324,"about_ca_system_score_gemma":0.00012325228,"threshold_uncertainty_score":0.018473923},"labels":[],"label_agreement":null},{"id":"W2114087169","doi":"10.1088/0004-637x/793/1/22","title":"A SUBMILLIMETER GALAXY ILLUMINATING ITS CIRCUMGALACTIC MEDIUM: Lyα SCATTERING IN A COLD, CLUMPY OUTFLOW","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"FP7 Space; Science and Technology Facilities Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Physics; Astrophysics; Galaxy; Interstellar medium; Astronomy; RADIUS; Outflow; H-alpha; Halo; Luminosity; Star formation; Line (geometry); Active galactic nucleus; Quasar; Emission spectrum; Spectral line","score_opus":0.00872514338178483,"score_gpt":0.21403190157496194,"score_spread":0.20530675819317712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114087169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938464,0.00007303694,0.0001156025,0.000011460703,0.0000013677302,0.0000016564159,0.000043641558,0.000011954195,0.0003566745],"genre_scores_gemma":[0.9995086,0.000035920384,0.00019486755,0.000027967619,0.0000058413425,0.0000015038536,0.00009534193,0.0000022353227,0.00012758757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999627,0.0000023400353,0.0000012109185,0.0000124735525,0.0000071287145,0.0000141689925],"domain_scores_gemma":[0.9998647,0.000014183393,0.000044631794,0.000010645192,0.000007647325,0.000058253983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007053917,0.00019606951,0.00015703985,0.0003505238,0.0002942036,0.00044145485,0.00021582654,0.00021647841,0.0006559438],"category_scores_gemma":[0.000117797936,0.00013079985,0.000082069055,0.00023129265,0.0002367016,0.00017467135,0.0004129164,0.00020487265,0.0002749211],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023524261,0.0000722133,0.6150399,0.00004955169,0.000037735135,0.003524296,0.001088771,0.00017429558,0.37116313,0.00017700286,0.00030015063,0.008137703],"study_design_scores_gemma":[0.000005633078,0.000110949084,0.992864,0.0000037339191,0.000011608567,0.0015988564,0.0002519696,0.00029585743,0.0042286385,0.000052188836,0.0005721116,0.000004362971],"about_ca_topic_score_codex":0.0018958154,"about_ca_topic_score_gemma":0.0034562207,"teacher_disagreement_score":0.0018958154,"about_ca_system_score_codex":0.00015654931,"about_ca_system_score_gemma":0.00006662643,"threshold_uncertainty_score":0.0037696362},"labels":[],"label_agreement":null},{"id":"W2114150813","doi":"10.1086/508487","title":"The Spatial Distribution of the Galactic First Stars. I. High‐Resolution<i>N</i>‐Body Approach","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Stars; Physics; Astrophysics; Milky Way; Galactic halo; Halo; Astronomy; Initial mass function; Star formation; Galaxy","score_opus":0.00570825634112755,"score_gpt":0.1888334550896735,"score_spread":0.18312519874854596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114150813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94788307,0.00028329607,0.0430636,0.00034210455,0.000019843936,0.00002154117,0.00042769455,0.00031250843,0.0076462156],"genre_scores_gemma":[0.9916044,0.00007585352,0.007280692,0.00005068281,0.000011170004,0.000012413725,0.0002772168,0.00004480068,0.00064290426],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998833,0.000027698892,0.0000042435518,0.00003776826,0.00002332814,0.000023518955],"domain_scores_gemma":[0.9995448,0.00011399209,0.00011051591,0.000115692834,0.00005810088,0.000056930123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042111982,0.00027650356,0.00037051053,0.00038620053,0.0004389604,0.0007903237,0.001340032,0.00072624773,0.0011949053],"category_scores_gemma":[0.002080824,0.00037453294,0.00079430646,0.0004895325,0.0005938165,0.0005668009,0.0007002168,0.00064460834,0.0003217149],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007457317,0.000037124028,0.040725913,0.000029283534,0.0000804263,0.0001276094,0.00008444254,0.9426107,0.004985501,0.0074088797,0.00036758432,0.0034680988],"study_design_scores_gemma":[0.00003448277,0.000021762038,0.010970232,0.000005620506,0.000021123411,0.00010835901,0.000029074039,0.9834235,0.0018533348,0.0027315516,0.00078639615,0.000014615887],"about_ca_topic_score_codex":0.011806448,"about_ca_topic_score_gemma":0.0054938165,"teacher_disagreement_score":0.011806448,"about_ca_system_score_codex":0.001023314,"about_ca_system_score_gemma":0.0004812445,"threshold_uncertainty_score":0.023475468},"labels":[],"label_agreement":null},{"id":"W2114163622","doi":"10.1088/0004-637x/767/2/122","title":"THE CLUSTERING OF GALAXIES IN THE SDSS-III BARYON OSCILLATION SPECTROSCOPIC SURVEY: LUMINOSITY AND COLOR DEPENDENCE AND REDSHIFT EVOLUTION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Science and Technology Facilities Council; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; University of Arizona; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Redshift; Galaxy; Luminosity; Redshift survey; Astronomy; Luminosity function; Luminous infrared galaxy","score_opus":0.008380689169209886,"score_gpt":0.21422330097120384,"score_spread":0.20584261180199395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114163622","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953426,0.000068152185,0.00039922836,0.00002521862,0.0000018709162,0.0000057501575,0.0033202788,0.000048886453,0.00078811496],"genre_scores_gemma":[0.98784864,0.00007670397,0.00080247235,0.000013363071,0.000008222721,0.000010520261,0.010727378,0.000019839536,0.0004928136],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974316,0.00004798631,0.000015898175,0.00006337734,0.00007362045,0.000056000812],"domain_scores_gemma":[0.9987005,0.00015124326,0.00060535804,0.00013311477,0.0001860482,0.00022361708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004195693,0.00025473986,0.00018375706,0.0016990104,0.0001779371,0.000352782,0.00022241593,0.0001769259,0.0007545099],"category_scores_gemma":[0.0012337657,0.00012706012,0.00023755532,0.0016830988,0.00022707388,0.00023832232,0.00051982515,0.0001924241,0.00054212863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003095777,0.000011168641,0.9948231,0.00000724491,0.000029076784,0.000012754345,0.000053305328,0.00056678546,0.0012362188,0.00007739263,0.00046746604,0.0026846505],"study_design_scores_gemma":[7.6862517e-7,0.0000043415293,0.99904734,0.0000012621949,0.0000028608426,0.000016111922,0.000018471896,0.0005930827,0.00012529544,0.000016724787,0.00017198722,0.0000016530781],"about_ca_topic_score_codex":0.021649953,"about_ca_topic_score_gemma":0.04267868,"teacher_disagreement_score":0.021649953,"about_ca_system_score_codex":0.00047390038,"about_ca_system_score_gemma":0.00020687704,"threshold_uncertainty_score":0.043047905},"labels":[],"label_agreement":null},{"id":"W2114262152","doi":"10.1088/0004-637x/773/2/91","title":"THE<i>EINSTEIN@HOME</i>SEARCH FOR RADIO PULSARS AND PSR J2007+2722 DISCOVERY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Smithsonian Astrophysical Observatory; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Max-Planck-Gesellschaft; Science and Technology Facilities Council; Fonds Québécois de la Recherche sur la Nature et les Technologies; National Radio Astronomy Observatory; Canarie; Canadian Institute for Advanced Research; California Institute of Technology; National Aeronautics and Space Administration; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Science Foundation","keywords":"Pulsar; Neutron star; Physics; Astronomy; Astrophysics","score_opus":0.010352795729856,"score_gpt":0.2947035019284461,"score_spread":0.2843507061985901,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114262152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.38526046,0.048920043,0.016669229,0.20148145,0.0041943723,0.00034754098,0.009953699,0.0043258467,0.32884738],"genre_scores_gemma":[0.77118605,0.02611012,0.04797056,0.029599167,0.009003583,0.0001575829,0.015353865,0.00071683596,0.0999022],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99975973,0.000045477103,0.000011158033,0.000037528684,0.000089780406,0.000056310855],"domain_scores_gemma":[0.99887353,0.00015164909,0.00024506275,0.00013920176,0.00014125722,0.0004493655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00088589813,0.00029895236,0.00015969876,0.0017893149,0.00066210877,0.0012372996,0.0003057282,0.00071994966,0.004876813],"category_scores_gemma":[0.0012172891,0.0001623401,0.00023570549,0.0016147278,0.0005649216,0.0009406696,0.0011894114,0.00064232823,0.0014720403],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002304919,0.00011125778,0.060890272,0.00021681703,0.00007135106,0.00088355696,0.0005712455,0.00036508718,0.00896955,0.035898674,0.4848221,0.40696964],"study_design_scores_gemma":[0.00004938516,0.00015190172,0.079008915,0.00012405367,0.000045412555,0.0007764584,0.00032958091,0.0005227377,0.004681123,0.0056801764,0.9085948,0.0000354847],"about_ca_topic_score_codex":0.0027299176,"about_ca_topic_score_gemma":0.005492519,"teacher_disagreement_score":0.004876813,"about_ca_system_score_codex":0.00094474823,"about_ca_system_score_gemma":0.0008681039,"threshold_uncertainty_score":0.016314566},"labels":[],"label_agreement":null},{"id":"W2114684312","doi":"10.1088/0004-637x/724/2/1396","title":"SUPERNOVA PTF 09UJ: A POSSIBLE SHOCK BREAKOUT FROM A DENSE CIRCUMSTELLAR WIND","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":199,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Light curve; Supernova; Ejecta; Astrophysics; Physics; Stars; Absolute magnitude; Astronomy","score_opus":0.008687349051530737,"score_gpt":0.22224410773864067,"score_spread":0.21355675868710994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114684312","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926845,0.0009331411,0.0024811642,0.00013327347,0.00008284945,0.000034947065,0.00015659083,0.00008471879,0.0034087943],"genre_scores_gemma":[0.99799216,0.00024214978,0.00066947204,0.00009447392,0.000063044805,0.0000062506215,0.00023401795,0.0000052203486,0.00069325854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999912,0.0000070428673,0.000008336552,0.000031535958,0.000012899794,0.000028225119],"domain_scores_gemma":[0.99980015,0.000022347946,0.000058542824,0.000021469357,0.000013934265,0.00008359427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024294545,0.000564562,0.00044984467,0.00044410554,0.0007594281,0.00083805807,0.00041320716,0.00091909117,0.0016256131],"category_scores_gemma":[0.0005148889,0.00025457935,0.00031233966,0.0002940519,0.00032270406,0.00035181522,0.0006998325,0.00061463274,0.00036686906],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013369285,0.00026680253,0.79801065,0.00016221823,0.00019634602,0.09440836,0.00041447586,0.0009157672,0.042094935,0.00534412,0.0016937681,0.055155627],"study_design_scores_gemma":[0.00031528538,0.0015361542,0.7896334,0.000084276435,0.00022432258,0.16116147,0.0004419831,0.0063306056,0.020357361,0.0034454616,0.016421512,0.000048215206],"about_ca_topic_score_codex":0.002364065,"about_ca_topic_score_gemma":0.0014468231,"teacher_disagreement_score":0.002364065,"about_ca_system_score_codex":0.0003744849,"about_ca_system_score_gemma":0.000168582,"threshold_uncertainty_score":0.005438268},"labels":[],"label_agreement":null},{"id":"W2114914177","doi":"10.1086/503273","title":"The Two Young Star Disks in the Central Parsec of the Galaxy: Properties, Dynamics, and Formation","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":696,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Stars; Parsec; Star formation; Luminosity function; Stellar mass; Luminosity; Young stellar object; Accretion (finance); Stellar density; Thick disk","score_opus":0.007709530957585328,"score_gpt":0.20541946325371876,"score_spread":0.19770993229613343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114914177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99848443,0.0005326044,0.00016325421,0.000016713133,0.0000011384357,0.0000017826083,0.00015361287,0.000008807017,0.000637672],"genre_scores_gemma":[0.9985526,0.0002309873,0.0003895932,0.0000121669345,0.000007001344,0.0000023738776,0.00048240813,0.000003836522,0.00031906113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999324,0.0000051400352,0.0000029199805,0.00002092285,0.0000168291,0.000021874243],"domain_scores_gemma":[0.99978644,0.000020614505,0.000085053056,0.000013478565,0.000029414216,0.000064907974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012283541,0.00020129397,0.00015608649,0.0008314593,0.00024824098,0.0005937353,0.00019887644,0.0001768387,0.0008031693],"category_scores_gemma":[0.00033909822,0.00013639509,0.00009359245,0.00043916027,0.00030721366,0.0004843569,0.00060837273,0.00014889924,0.0002959292],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013857606,0.000056590336,0.9609896,0.00005978482,0.000023226974,0.00022700275,0.00053005875,0.0003398642,0.02116287,0.00040094854,0.0003214336,0.015749963],"study_design_scores_gemma":[0.0000041730405,0.00005183386,0.9962525,0.000005319178,0.000010558453,0.000465951,0.00008749438,0.0005349806,0.0012903034,0.00010937111,0.0011816762,0.0000057493903],"about_ca_topic_score_codex":0.0025670095,"about_ca_topic_score_gemma":0.0035309722,"teacher_disagreement_score":0.0025670095,"about_ca_system_score_codex":0.00020378691,"about_ca_system_score_gemma":0.00014398323,"threshold_uncertainty_score":0.0051041245},"labels":[],"label_agreement":null},{"id":"W2114962824","doi":"10.1088/0004-637x/742/2/129","title":"IMPACTS OF DARK STARS ON REIONIZATION AND SIGNATURES IN THE COSMIC MICROWAVE BACKGROUND","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Reionization; Physics; Astrophysics; Cosmic microwave background; Stars; Dark matter; Astronomy; Anisotropy; Redshift; Galaxy","score_opus":0.017598070310733797,"score_gpt":0.22910676046560352,"score_spread":0.21150869015486973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2114962824","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954666,0.00044131532,0.0017000054,0.0000625406,0.000006159069,0.0000068101713,0.0008025598,0.000086008,0.001427962],"genre_scores_gemma":[0.9978453,0.00017211023,0.0007066576,0.000015503694,0.0000055884607,0.0000031947152,0.00089336873,0.000043171538,0.00031511395],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997943,0.000038320304,0.000009248008,0.00006318504,0.000037406564,0.000057527508],"domain_scores_gemma":[0.99892884,0.00030074007,0.00029045888,0.00018228007,0.00009885156,0.00019888494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049792277,0.0007397844,0.00044236964,0.0009983581,0.0002848871,0.0010085428,0.00046060764,0.00042386816,0.0011761407],"category_scores_gemma":[0.0020670148,0.00026370856,0.0006662726,0.00089318055,0.0003621149,0.0007750357,0.00088543154,0.00043819574,0.0002505663],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030169473,0.00006274527,0.7954715,0.00011359631,0.00039074532,0.0007051738,0.0001379499,0.1710542,0.013331921,0.0052755573,0.00066701125,0.012487865],"study_design_scores_gemma":[0.000057953865,0.00019500927,0.6663253,0.000069968395,0.00022875152,0.00046531725,0.00028699051,0.30654332,0.016188791,0.004839018,0.0047060293,0.000093614835],"about_ca_topic_score_codex":0.0059594894,"about_ca_topic_score_gemma":0.0039252443,"teacher_disagreement_score":0.0059594894,"about_ca_system_score_codex":0.0004965495,"about_ca_system_score_gemma":0.00027564497,"threshold_uncertainty_score":0.011849582},"labels":[],"label_agreement":null},{"id":"W2115171714","doi":"10.1088/0004-637x/786/1/2","title":"TRANSIT CONFIRMATION AND IMPROVED STELLAR AND PLANET PARAMETERS FOR THE SUPER-EARTH HD 97658 b AND ITS HOST STAR","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Planet; Astrophysics; Photometry (optics); Stars; Parallax; Transit (satellite); Spitzer Space Telescope; Astronomy; Star (game theory); Super-Earth; RADIUS; Planetary system","score_opus":0.010956327855321446,"score_gpt":0.20417992962605597,"score_spread":0.19322360177073453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115171714","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998387,0.000062692976,0.00030664416,0.000012489365,0.0000026242274,0.0000031897684,0.00034299996,0.000011710539,0.0008707532],"genre_scores_gemma":[0.9980672,0.000032339387,0.00046855255,0.00001000715,0.0000038785493,0.000001851866,0.0010925928,0.0000051921716,0.00031835755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991,0.0000076759925,0.000008545942,0.000033174634,0.000019363997,0.000021269441],"domain_scores_gemma":[0.99953413,0.000065171924,0.00017615543,0.00006210889,0.000078829005,0.0000836623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002861125,0.00019620941,0.0001328941,0.0008238342,0.0002852763,0.00043943204,0.00013903434,0.00017377414,0.0020367526],"category_scores_gemma":[0.00044620413,0.000075743155,0.00016610212,0.0004362431,0.00014082118,0.00028444335,0.0002977625,0.00018432968,0.00045164613],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034217394,0.000040184317,0.9419128,0.000038456536,0.000039594008,0.00025526673,0.00028489067,0.00027992792,0.046475884,0.0002963731,0.0002453266,0.0097892145],"study_design_scores_gemma":[0.00000991392,0.00005103218,0.99281013,0.000007470307,0.000026392483,0.00019461164,0.00022453173,0.0008481105,0.0046853633,0.00007313599,0.0010650195,0.0000043194887],"about_ca_topic_score_codex":0.0029930964,"about_ca_topic_score_gemma":0.0063064084,"teacher_disagreement_score":0.0029930964,"about_ca_system_score_codex":0.00017661777,"about_ca_system_score_gemma":0.0001406938,"threshold_uncertainty_score":0.0068135858},"labels":[],"label_agreement":null},{"id":"W2115179958","doi":"10.1088/0004-637x/778/2/104","title":"COMPARING THE WHITE DWARF COOLING SEQUENCES IN 47 Tuc AND NGC 6397","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"White dwarf; Globular cluster; Metallicity; Hubble space telescope; Blue dwarf; Proper motion; Stellar atmosphere; Stellar evolution","score_opus":0.017311338730726284,"score_gpt":0.22671512209490538,"score_spread":0.20940378336417909,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115179958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987606,0.000016457629,0.00003893825,0.000007169634,9.819398e-7,0.0000010797352,0.00016404624,0.000007803775,0.0010029874],"genre_scores_gemma":[0.9982768,0.00002621603,0.0001680597,0.000006336026,0.0000019328322,0.0000035490298,0.0012124893,0.000011032862,0.0002935562],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984765,0.000008335237,0.000010477476,0.000035331144,0.000039171395,0.00005897227],"domain_scores_gemma":[0.99898344,0.0001751843,0.00022733642,0.00015102145,0.0001819878,0.00028107315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019012141,0.00010710642,0.00022495903,0.0021207954,0.00060911046,0.00067894644,0.00028706912,0.0002576453,0.0012508252],"category_scores_gemma":[0.000947657,0.00011908284,0.00025173678,0.0019431129,0.00039005483,0.00017807848,0.00053124176,0.0002664258,0.00043750144],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051401416,0.00004143264,0.9506902,0.000021498396,0.00006622559,0.0005815446,0.0018080827,0.0011072315,0.02896283,0.0011499198,0.00067015056,0.014386939],"study_design_scores_gemma":[0.0000035251455,0.000011068233,0.99844956,0.0000032723688,0.000005457848,0.00007248034,0.00023617782,0.00028591478,0.00049355795,0.00008419486,0.0003519321,0.0000028712852],"about_ca_topic_score_codex":0.05407678,"about_ca_topic_score_gemma":0.07853092,"teacher_disagreement_score":0.05407678,"about_ca_system_score_codex":0.00091177115,"about_ca_system_score_gemma":0.00043724125,"threshold_uncertainty_score":0.10752404},"labels":[],"label_agreement":null},{"id":"W2115238770","doi":"10.1088/0004-637x/710/1/51","title":"THE MASS-METALLICITY RELATION OF GLOBULAR CLUSTERS IN THE CONTEXT OF NONLINEAR COLOR-METALLICTY RELATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Metallicity; Context (archaeology); Scaling; Galaxy; Cluster (spacecraft); Luminosity; Elliptical galaxy","score_opus":0.006502876554090187,"score_gpt":0.2161039793769235,"score_spread":0.2096011028228333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115238770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99739265,0.000037827478,0.0012388789,0.0000868286,0.0000021461303,0.000009408365,0.00008326995,0.000023045124,0.0011259889],"genre_scores_gemma":[0.9989133,0.000029860612,0.00070971384,0.000014979302,0.0000018234033,0.0000072843336,0.000081029495,0.000010279162,0.00023181963],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983704,0.000060227274,0.0000069203293,0.00004055656,0.000021213154,0.0000339692],"domain_scores_gemma":[0.9987618,0.00060691696,0.00020871816,0.00017413478,0.00010873978,0.00013981771],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067273865,0.00035310484,0.00029946413,0.0005048376,0.0005042816,0.0008578153,0.000674797,0.0004891465,0.0012954929],"category_scores_gemma":[0.0037591099,0.00018916144,0.00032070893,0.00047819788,0.0011298368,0.00073670404,0.0008031169,0.00044551265,0.00012371068],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016567114,0.000086075706,0.16778184,0.000037029207,0.00006151301,0.00017104506,0.000487082,0.80894285,0.0038895684,0.015137564,0.00056833157,0.002671541],"study_design_scores_gemma":[0.00007740277,0.000119458644,0.06888867,0.000016004406,0.00003179804,0.00011012552,0.00026649068,0.90967023,0.0013532313,0.018591085,0.0008425583,0.0000328709],"about_ca_topic_score_codex":0.011564198,"about_ca_topic_score_gemma":0.010825028,"teacher_disagreement_score":0.011564198,"about_ca_system_score_codex":0.0011684591,"about_ca_system_score_gemma":0.00038106824,"threshold_uncertainty_score":0.022993743},"labels":[],"label_agreement":null},{"id":"W2115611172","doi":"10.1088/0004-637x/742/1/31","title":"LONG-TERM X-RAY MONITORING OF THE YOUNG PULSAR PSR B1509–58","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Magnetar; Astrophysics; Physics; Flux (metallurgy); X-ray pulsar; Neutron star; Static timing analysis; Dipole; X-ray; Astronomy; Nuclear physics","score_opus":0.024700186904696244,"score_gpt":0.30855016097138865,"score_spread":0.28384997406669243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115611172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918705,0.000104903884,0.00018774605,0.000008558386,0.0000017770402,0.0000042500783,0.0001277135,0.000011292717,0.0003668057],"genre_scores_gemma":[0.99832207,0.00012928514,0.0006360246,0.000016953845,0.000008850164,0.000010018425,0.00066258974,0.000007264432,0.00020692537],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998994,0.000009437589,0.000013894006,0.00003090892,0.000031668893,0.0000146023995],"domain_scores_gemma":[0.9995449,0.00004681056,0.00022864122,0.00003344717,0.000076073775,0.00007010791],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026923133,0.00013518677,0.0002605809,0.00065386354,0.00018767643,0.00023218551,0.00021154924,0.00019058915,0.00032283852],"category_scores_gemma":[0.0006186176,0.00011713405,0.000105236926,0.00035418573,0.00015071177,0.0002544539,0.00033259223,0.00020891715,0.00023410501],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026544847,0.00008104991,0.80085194,0.00006125429,0.00007465692,0.00047186832,0.00023215974,0.00054251764,0.17608708,0.00013758971,0.00027323098,0.020921137],"study_design_scores_gemma":[0.0000065848176,0.00011330556,0.9958604,0.000006565529,0.000017254286,0.00026921887,0.00003903044,0.00050840795,0.0026644298,0.000027971639,0.00048312338,0.0000035592282],"about_ca_topic_score_codex":0.0011877776,"about_ca_topic_score_gemma":0.0020599274,"teacher_disagreement_score":0.0011877776,"about_ca_system_score_codex":0.00013082368,"about_ca_system_score_gemma":0.00008230402,"threshold_uncertainty_score":0.0023617744},"labels":[],"label_agreement":null},{"id":"W2115698923","doi":"10.1088/0004-637x/736/2/110","title":"AEGIS: THE MORPHOLOGIES OF GREEN GALAXIES AT 0.4 &lt;<i>z</i>&lt; 1.2","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Elliptical galaxy; Galaxy; Galaxy group; Lenticular galaxy; Luminous infrared galaxy; Population; Peculiar galaxy; Star formation","score_opus":0.01625116165793865,"score_gpt":0.20613236030799822,"score_spread":0.18988119865005956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115698923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99354255,0.00007300298,0.00015158224,0.00004019235,0.0000032452067,0.0000064592514,0.0031470035,0.00008437031,0.0029516385],"genre_scores_gemma":[0.994148,0.000050522227,0.0004538342,0.000034492743,0.0000052584596,0.000006234448,0.004330459,0.0000339022,0.00093729625],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995923,0.0000023989257,0.0000013052911,0.000010115971,0.0000067519927,0.000020106963],"domain_scores_gemma":[0.99976164,0.000013542925,0.0000796703,0.000018225108,0.000031001924,0.000095958705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009411834,0.00016568105,0.00012703128,0.0015013346,0.00021351692,0.00045294172,0.00017280308,0.00014787441,0.002054289],"category_scores_gemma":[0.00019415964,0.000088975146,0.00018022551,0.00061354873,0.00023794045,0.00024525487,0.00034249795,0.00018464949,0.00047759974],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001891735,0.000029655532,0.9693262,0.000019963742,0.000044547996,0.00016567191,0.00041716083,0.00059756386,0.01405648,0.0007389178,0.004084303,0.010330346],"study_design_scores_gemma":[0.0000028354025,0.0000071144,0.99863833,0.0000019270376,0.0000030095407,0.000037983238,0.000091591,0.0002627751,0.00025102263,0.00005058116,0.00065127,0.0000015082394],"about_ca_topic_score_codex":0.013717616,"about_ca_topic_score_gemma":0.024525996,"teacher_disagreement_score":0.013717616,"about_ca_system_score_codex":0.0003795886,"about_ca_system_score_gemma":0.000098546916,"threshold_uncertainty_score":0.027275562},"labels":[],"label_agreement":null},{"id":"W2115708669","doi":"10.1088/0004-637x/775/2/138","title":"SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS. VII. THE SUBSTELLAR MASS FUNCTION REVISITED","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Brown dwarf; Astrometry; Initial mass function; Stellar mass; Mass distribution; Low Mass; Cluster (spacecraft); Function (biology); Line (geometry)","score_opus":0.007339441583730753,"score_gpt":0.20634179910710518,"score_spread":0.19900235752337442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115708669","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99158406,0.0032417267,0.0024782745,0.00021674238,0.000013940372,0.0000036402728,0.00011305294,0.00004756623,0.0023010338],"genre_scores_gemma":[0.9989417,0.0003813903,0.00031213008,0.000026541053,0.000008732383,0.0000011011582,0.000054489665,0.0000045303054,0.000269407],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992037,0.000013041361,0.000005915182,0.000027772818,0.000016495167,0.000016373451],"domain_scores_gemma":[0.9995695,0.0001299642,0.00012533665,0.000053457796,0.000057355886,0.000064426225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033317204,0.00020460776,0.00018526461,0.0011592419,0.00032062794,0.0007191303,0.00038292856,0.0004350328,0.0010181464],"category_scores_gemma":[0.0009255083,0.000078198595,0.00021584403,0.0008957594,0.0006877738,0.00064638566,0.00040906528,0.00028376296,0.00028304124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014744286,0.000012069076,0.93172336,0.00008607848,0.000059042904,0.0010330396,0.0008889374,0.002048941,0.009104623,0.0073114317,0.00060659036,0.046978593],"study_design_scores_gemma":[0.000004621171,0.000051558814,0.98359007,0.000028373566,0.000029152157,0.0017242212,0.00054754235,0.0038467587,0.0020923512,0.0057807793,0.0022932976,0.000011151854],"about_ca_topic_score_codex":0.011430413,"about_ca_topic_score_gemma":0.009062211,"teacher_disagreement_score":0.011430413,"about_ca_system_score_codex":0.00054330705,"about_ca_system_score_gemma":0.00020865876,"threshold_uncertainty_score":0.022727787},"labels":[],"label_agreement":null},{"id":"W2115716286","doi":"10.1088/0004-637x/747/1/82","title":"THERMAL PHASE VARIATIONS OF WASP-12b: DEFYING PREDICTIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":207,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Amplitude; Opacity; Geometric albedo; Planet; Transit (satellite); Astrophysics; Monte Carlo method; Computational physics; Optics; Stars; Photometry (optics); Mathematics","score_opus":0.017127984889081082,"score_gpt":0.25477696668017663,"score_spread":0.23764898179109556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115716286","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997051,0.00008732459,0.0015931891,0.00003722695,0.0000036024055,0.0000047222848,0.00014194564,0.00007635342,0.0010047178],"genre_scores_gemma":[0.9990889,0.000024492643,0.00056686177,0.0000055246815,0.0000028432764,0.0000034203042,0.00017591199,0.000012289626,0.00011969962],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992824,0.000007966972,0.000001917813,0.000023458118,0.000021536565,0.00001689111],"domain_scores_gemma":[0.9998079,0.000038285685,0.00005884027,0.000027981196,0.000037997488,0.000028910355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014306493,0.00023152809,0.00020901259,0.00033498488,0.00030897046,0.00029832398,0.00037926613,0.00025678723,0.00070563884],"category_scores_gemma":[0.00063199835,0.00020563044,0.00017734579,0.00032769676,0.0004233632,0.00030537279,0.00035173693,0.0004248184,0.00018710019],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002301849,0.0001096882,0.41530403,0.0001371385,0.00010356141,0.00076386856,0.00056759286,0.038757853,0.515679,0.0017676867,0.00078068813,0.023727011],"study_design_scores_gemma":[0.000090363916,0.00046655638,0.8343855,0.000014076734,0.00006378715,0.0005904275,0.00017768216,0.08969631,0.06984519,0.0019413505,0.0026813322,0.00004744238],"about_ca_topic_score_codex":0.0026087873,"about_ca_topic_score_gemma":0.0024841086,"teacher_disagreement_score":0.0026087873,"about_ca_system_score_codex":0.0004468669,"about_ca_system_score_gemma":0.000108464556,"threshold_uncertainty_score":0.005187154},"labels":[],"label_agreement":null},{"id":"W2115962205","doi":"10.1088/0004-637x/738/2/125","title":"MODELING OF THE HERMES SUBMILLIMETER SOURCE LENSED BY A DARK MATTER DOMINATED FOREGROUND GROUP OF GALAXIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; University of British Columbia","funders":"Science and Technology Facilities Council; Centre National de la Recherche Scientifique; National Astronomical Observatories, Chinese Academy of Sciences; Max-Planck-Gesellschaft; Università degli Studi di Padova; Cardiff University; University of Sussex; National Aeronautics and Space Administration; Imperial College London; University of Lethbridge; California Institute of Technology; Centre National d’Etudes Spatiales; W. M. Keck Foundation","keywords":"Physics; Astrophysics; Einstein radius; Galaxy; Dark matter; Redshift; Velocity dispersion; Gravitational lens; RADIUS; Plateau de Bure Interferometer; Population; Dark matter halo; Halo","score_opus":0.0097093763026881,"score_gpt":0.19010924774984075,"score_spread":0.18039987144715267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2115962205","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98662275,0.00012392344,0.00848613,0.0001503172,0.0000030697565,0.000026394313,0.00043282914,0.0000810082,0.0040735286],"genre_scores_gemma":[0.99523443,0.00009333218,0.0021878518,0.00003017934,0.000011353013,0.00002064807,0.00040885762,0.000020543617,0.001992779],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998635,0.000030000476,0.000005780204,0.00004160112,0.000021144055,0.000038055125],"domain_scores_gemma":[0.9995241,0.0001313387,0.00017285021,0.000033244796,0.000042733147,0.000095624964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003791604,0.0006319234,0.00041804224,0.0007557617,0.00032396018,0.0007340505,0.0008514119,0.0005416506,0.0018128891],"category_scores_gemma":[0.00096814195,0.0002907044,0.0005685358,0.00040313802,0.00037499506,0.0006410897,0.0004986787,0.00022335075,0.0003534706],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017713146,0.000045115376,0.110649824,0.00003053515,0.0001019835,0.0003398719,0.00025941982,0.87082845,0.0035886744,0.0077852234,0.0005419517,0.0056517515],"study_design_scores_gemma":[0.000024965571,0.000048135204,0.030044982,0.0000061121514,0.000029139735,0.000070523434,0.0001023075,0.96656024,0.0004156459,0.0021351497,0.00054986787,0.000012990663],"about_ca_topic_score_codex":0.091322884,"about_ca_topic_score_gemma":0.045514423,"teacher_disagreement_score":0.091322884,"about_ca_system_score_codex":0.0019053755,"about_ca_system_score_gemma":0.00060831534,"threshold_uncertainty_score":0.18158269},"labels":[],"label_agreement":null},{"id":"W2116009256","doi":"10.1086/527351","title":"The On/Off Nature of Star‐Planet Interactions","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":282,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Stars; Longitude; Starspot; Stellar rotation; Spectral line; Observable; Orbit (dynamics); Jupiter (rocket family); Rotation period","score_opus":0.009587294084236352,"score_gpt":0.23336635284024124,"score_spread":0.22377905875600487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116009256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997027,0.000098765864,0.00015520859,0.00001499238,0.000002948874,0.000003894482,0.00009767062,0.000010086471,0.002589389],"genre_scores_gemma":[0.9993037,0.00004352468,0.00008430916,0.000015522459,0.0000055711853,0.0000023952323,0.00021284466,0.000003060062,0.0003291523],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981564,0.00002436452,0.000012100162,0.00005091361,0.000054360422,0.000042598986],"domain_scores_gemma":[0.9991648,0.00019996609,0.00031607275,0.00009064277,0.00009031927,0.00013819974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015417773,0.000120401164,0.00015832085,0.0005976497,0.0002788313,0.0005670081,0.00023819762,0.00022562232,0.0018103411],"category_scores_gemma":[0.00083659677,0.000106204316,0.00012543568,0.00031913968,0.0003028521,0.00034094075,0.0005263138,0.00020938998,0.00025617052],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027205853,0.00008346928,0.91196984,0.00005624427,0.000078129226,0.00042763585,0.0005993382,0.00024632178,0.05721318,0.00033882362,0.0002763136,0.02843866],"study_design_scores_gemma":[0.0000013245663,0.000049692604,0.99772173,0.0000027575572,0.0000054098223,0.0002701744,0.0001568031,0.00017456769,0.0010136756,0.00008448508,0.0005171246,0.0000022574002],"about_ca_topic_score_codex":0.00091666915,"about_ca_topic_score_gemma":0.0018405188,"teacher_disagreement_score":0.0018103411,"about_ca_system_score_codex":0.00019739814,"about_ca_system_score_gemma":0.000086181346,"threshold_uncertainty_score":0.0060561895},"labels":[],"label_agreement":null},{"id":"W2116035233","doi":"10.1088/0004-637x/765/1/55","title":"OBSERVATION OF COSMIC-RAY ANISOTROPY WITH THE ICETOP AIR SHOWER ARRAY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Air shower; Cosmic ray; Physics; Anisotropy; Neutrino; Amplitude; Astrophysics; Ultra-high-energy cosmic ray; Detector; Nuclear physics; Optics","score_opus":0.008759624915070425,"score_gpt":0.20111816158525977,"score_spread":0.19235853667018935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116035233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98955256,0.00022833043,0.0012244439,0.000057858688,0.00001657728,0.000016001804,0.0023327905,0.000073178184,0.006498245],"genre_scores_gemma":[0.99176896,0.00022485782,0.002713545,0.000042116455,0.00004294336,0.00001232845,0.004527279,0.000044073102,0.0006238862],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996916,0.000030309759,0.000010242064,0.00007798765,0.00011313671,0.00007675939],"domain_scores_gemma":[0.9988593,0.00019083488,0.00041154225,0.00017932733,0.00023360782,0.00012538528],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039004293,0.00028465714,0.00037329923,0.0010572738,0.00036257692,0.00050249475,0.00028842874,0.00024080329,0.0007543036],"category_scores_gemma":[0.0008056401,0.00021644971,0.0002595279,0.0010733999,0.00028168233,0.00035445613,0.0004927144,0.0005702426,0.00024157137],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009956443,0.00019437335,0.8327589,0.00009551177,0.0002978878,0.00092088064,0.0003826356,0.0018247552,0.13636754,0.0009154587,0.003524122,0.02172233],"study_design_scores_gemma":[0.000018559947,0.000115792674,0.9791612,0.000011072615,0.000047778874,0.00071278017,0.00007102607,0.0021920896,0.013399196,0.0001275752,0.0041250847,0.000017945978],"about_ca_topic_score_codex":0.0043113893,"about_ca_topic_score_gemma":0.012588297,"teacher_disagreement_score":0.0043113893,"about_ca_system_score_codex":0.00030865718,"about_ca_system_score_gemma":0.0002275095,"threshold_uncertainty_score":0.008572578},"labels":[],"label_agreement":null},{"id":"W2116285186","doi":"10.1088/0004-637x/787/1/19","title":"THE PAndAS FIELD OF STREAMS: STELLAR STRUCTURES IN THE MILKY WAY HALO TOWARD ANDROMEDA AND TRIANGULUM","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Globular cluster; Galactic halo; Halo; Stellar collision; Metallicity; Stellar density; Star cluster; Local Group; Dwarf galaxy","score_opus":0.009311883153715587,"score_gpt":0.23132541715682808,"score_spread":0.2220135340031125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116285186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99755967,0.000116825664,0.0001443532,0.000028361117,0.000002784036,0.0000060434077,0.00043247806,0.0000374446,0.0016719948],"genre_scores_gemma":[0.9979809,0.000068255074,0.00069667527,0.000013719441,0.0000074622326,0.000004255122,0.0008929642,0.000010733939,0.0003249873],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989974,0.000014059773,0.0000031753898,0.000036181995,0.000020250709,0.000026563795],"domain_scores_gemma":[0.9998104,0.00001599411,0.00006323947,0.000021686865,0.000024084397,0.00006457969],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017301989,0.00018044647,0.00014659837,0.0013797501,0.00045946948,0.0005795159,0.00021700248,0.00012118395,0.0012541082],"category_scores_gemma":[0.00034344403,0.00009827355,0.00013484417,0.00094854855,0.0002361723,0.00020933627,0.0008183647,0.000111989284,0.0003127118],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002718059,0.000042690765,0.9533365,0.00004083227,0.000058336547,0.00034953846,0.0011334241,0.0005260193,0.011471271,0.00085898023,0.0010865406,0.030824102],"study_design_scores_gemma":[0.00001135071,0.000029838078,0.9948125,0.000011381799,0.000012719081,0.00025572695,0.00066480273,0.00058922556,0.0004457253,0.00013616924,0.0030242046,0.000006386474],"about_ca_topic_score_codex":0.0143026775,"about_ca_topic_score_gemma":0.02744477,"teacher_disagreement_score":0.0143026775,"about_ca_system_score_codex":0.00022355019,"about_ca_system_score_gemma":0.00026664662,"threshold_uncertainty_score":0.028438866},"labels":[],"label_agreement":null},{"id":"W2116312019","doi":"10.1088/0004-637x/746/1/85","title":"THE<i>HUBBLE SPACE TELESCOPE</i>CLUSTER SUPERNOVA SURVEY. V. IMPROVING THE DARK-ENERGY CONSTRAINTS ABOVE<i>z</i>&gt; 1 AND BUILDING AN EARLY-TYPE-HOSTED SUPERNOVA SAMPLE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1704,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Waterloo","funders":"Japan Society for the Promotion of Science; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution","keywords":"Physics; Dark energy; Astrophysics; Redshift; Photometry (optics); Supernova; Galaxy; Hubble's law; Astronomy; Cosmology; Stars","score_opus":0.01361123272233618,"score_gpt":0.2356801487675814,"score_spread":0.2220689160452452,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116312019","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3842883,0.006218614,0.0054969746,0.0070265313,0.0010267609,0.0006102113,0.5255706,0.0016496547,0.06811237],"genre_scores_gemma":[0.45894626,0.0035466626,0.020216685,0.0016543586,0.0006727396,0.0005081537,0.48048127,0.00045519642,0.033518765],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973875,0.0000362983,0.00002033024,0.000050170485,0.00009754831,0.000056793604],"domain_scores_gemma":[0.99683493,0.0001458965,0.0006279716,0.000365224,0.0007381363,0.001287699],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016700267,0.00037253607,0.0003300819,0.0060848854,0.0006283012,0.0009460972,0.00053876307,0.00031668227,0.0043650856],"category_scores_gemma":[0.0019127886,0.00023080404,0.00034643736,0.0029907993,0.00021007769,0.0005700521,0.0009662165,0.00055105845,0.0021759102],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045362208,0.00018721238,0.5197487,0.00030060278,0.00028485578,0.00016871344,0.00031359625,0.00094512716,0.0060715186,0.0063760476,0.35965723,0.10549277],"study_design_scores_gemma":[0.000059244907,0.00004387752,0.8746084,0.00009106689,0.00004550061,0.00006326261,0.0001322719,0.00051200564,0.00096035545,0.0008147865,0.12265092,0.000018231503],"about_ca_topic_score_codex":0.124888934,"about_ca_topic_score_gemma":0.21744281,"teacher_disagreement_score":0.124888934,"about_ca_system_score_codex":0.0018520611,"about_ca_system_score_gemma":0.003359946,"threshold_uncertainty_score":0.24832398},"labels":[],"label_agreement":null},{"id":"W2116346848","doi":"10.1086/512544","title":"VLA and <i>XMM-Newton</i> Observations of the SNR W41/TeV Gamma-Ray Source HESS J1834-087","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Molecular cloud; Galactic plane; Supernova remnant; RADIUS; Supernova; Galactic Center; Range (aeronautics); Radial velocity","score_opus":0.011175743705942421,"score_gpt":0.21492166517653583,"score_spread":0.2037459214705934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116346848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967805,0.00007223197,0.000096837444,0.0000296563,0.0000032470075,0.0000049342625,0.0007767132,0.00003462976,0.0022012885],"genre_scores_gemma":[0.9926916,0.00017208153,0.0013725492,0.00005241043,0.000021066373,0.0000149490415,0.004299301,0.000024310528,0.0013517833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999298,0.0000048652687,0.000006424629,0.000016075695,0.000024547317,0.00001829669],"domain_scores_gemma":[0.999818,0.000012710784,0.00005690752,0.000022673148,0.000031141735,0.000058710826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014269953,0.00015629888,0.00017055357,0.0009845776,0.00021955486,0.0003929516,0.00020095108,0.0002638348,0.0011760729],"category_scores_gemma":[0.00019437562,0.00017467936,0.00017504935,0.0005770082,0.00010965089,0.00017558025,0.000340235,0.00019659405,0.00052950624],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005581602,0.00019424414,0.6955883,0.0000951531,0.00017830812,0.002481322,0.0008400976,0.0010970342,0.26208562,0.0005221595,0.0036305215,0.032729115],"study_design_scores_gemma":[0.000010228468,0.000029343746,0.99522203,0.000006786677,0.000014806554,0.0002828412,0.00006591094,0.00058715855,0.0022166825,0.000035696918,0.0015227111,0.0000057482766],"about_ca_topic_score_codex":0.005469091,"about_ca_topic_score_gemma":0.011276862,"teacher_disagreement_score":0.005469091,"about_ca_system_score_codex":0.00023062367,"about_ca_system_score_gemma":0.00008137968,"threshold_uncertainty_score":0.01087451},"labels":[],"label_agreement":null},{"id":"W2116536024","doi":"10.1088/0004-637x/732/1/18","title":"TIME-INTEGRATED SEARCHES FOR POINT-LIKE SOURCES OF NEUTRINOS WITH THE 40-STRING IceCube DETECTOR","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":171,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Sky; Neutrino; Physics; Muon; Neutrino detector; Detector; Point source; Neutrino astronomy; Astrophysics; Astronomy; String (physics); Particle physics; Neutrino oscillation; Optics","score_opus":0.01635363753172925,"score_gpt":0.21107392607057107,"score_spread":0.19472028853884182,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116536024","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9760582,0.0006108443,0.0060627596,0.00005841976,0.000016601492,0.000047255377,0.008913155,0.00037351242,0.007859236],"genre_scores_gemma":[0.91157943,0.00070910534,0.042307593,0.0000640849,0.000054863154,0.00011086361,0.041293763,0.00011584241,0.0037644573],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995229,0.00009422991,0.000020499967,0.00013622877,0.00015304536,0.00007308732],"domain_scores_gemma":[0.9994875,0.0001393943,0.00013494564,0.000067442816,0.00009366562,0.00007698613],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00085037405,0.0005589579,0.0006680288,0.0012809121,0.00026269403,0.00075287774,0.0005961975,0.00028623175,0.0023133515],"category_scores_gemma":[0.0010177017,0.00028175884,0.000584614,0.0020285037,0.00024517794,0.00059484947,0.00077569735,0.00027392738,0.00050878077],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.006405251,0.00044109783,0.6558324,0.0004993748,0.0019491208,0.0011912663,0.0004650146,0.07919759,0.105925195,0.004528414,0.009423293,0.13414198],"study_design_scores_gemma":[0.00036362963,0.0016568706,0.7333825,0.00009665703,0.0007393568,0.0019207951,0.00044284412,0.14532655,0.0739108,0.0061969175,0.035760004,0.00020310529],"about_ca_topic_score_codex":0.0042872187,"about_ca_topic_score_gemma":0.010190016,"teacher_disagreement_score":0.0042872187,"about_ca_system_score_codex":0.00051482336,"about_ca_system_score_gemma":0.00062705297,"threshold_uncertainty_score":0.008524537},"labels":[],"label_agreement":null},{"id":"W2116696835","doi":"10.1086/308545","title":"The Cosmic‐Ray Electron and Positron Spectra Measured at 1 AU during Solar Minimum Activity","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":253,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Positron; Cosmic ray; Electron; Spectrometer; Spectral line; PAMELA detector; Electron spectrometer; Nuclear physics; Astronomy; Optics; Ultra-high-energy cosmic ray; Cathode ray","score_opus":0.0042523870156273205,"score_gpt":0.20156422928415532,"score_spread":0.197311842268528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116696835","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99709654,0.00018495588,0.0002288202,0.000021568532,0.0000077410195,0.000006431469,0.00042746423,0.000028887715,0.001997557],"genre_scores_gemma":[0.9974987,0.00012493061,0.000758778,0.000015680638,0.000013917856,0.0000097777565,0.00094642636,0.000017971153,0.00061382813],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989367,0.000009872011,0.0000035657108,0.000028639888,0.000039517352,0.000024715393],"domain_scores_gemma":[0.999811,0.000033945067,0.00004118269,0.000014855533,0.00006622054,0.000032749143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014600312,0.00029680933,0.00031217773,0.0008631866,0.000581541,0.00045294323,0.00032416903,0.00034259525,0.00085795595],"category_scores_gemma":[0.00041200517,0.00019769634,0.00016639476,0.0005056064,0.0001801307,0.00027154706,0.000338583,0.00031568512,0.00020364374],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016943945,0.00018386163,0.6308912,0.00013878128,0.00021019577,0.001272867,0.0014614981,0.0008106521,0.33320013,0.00041743624,0.0009480326,0.028770993],"study_design_scores_gemma":[0.000015614924,0.00015860649,0.98189837,0.000007240667,0.000035171757,0.00025773878,0.00009988361,0.0008519168,0.014030767,0.0000470115,0.0025864255,0.000011396819],"about_ca_topic_score_codex":0.0060606664,"about_ca_topic_score_gemma":0.01820796,"teacher_disagreement_score":0.0060606664,"about_ca_system_score_codex":0.00040192791,"about_ca_system_score_gemma":0.00014542803,"threshold_uncertainty_score":0.012050748},"labels":[],"label_agreement":null},{"id":"W2116712222","doi":"10.1086/341617","title":"Eccentricity Excitation and Apsidal Resonance Capture in the Planetary System υ Andromedae","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Apsidal precession; Physics; Planet; Astrophysics; Precession; Eccentricity (behavior); Orbital eccentricity; Astronomy; Planetary system; Celestial mechanics; Outer planets","score_opus":0.010946624722353058,"score_gpt":0.19527322316816104,"score_spread":0.18432659844580798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116712222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993112,0.000043536424,0.000042700623,0.000011600278,5.903395e-7,8.595109e-7,0.000016197162,0.0000034087748,0.00056993135],"genre_scores_gemma":[0.99979657,0.000018530034,0.00004371829,0.0000049982623,9.488558e-7,7.612123e-7,0.000026201309,0.0000012237535,0.0001070679],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999498,0.000009164434,0.000003021061,0.00001692981,0.000010277873,0.000010837133],"domain_scores_gemma":[0.9998042,0.00004090661,0.000088086774,0.00001867804,0.000012782365,0.000035424244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012086946,0.0001119438,0.00012397839,0.00035993799,0.0003258127,0.000373791,0.00018422178,0.00020610448,0.0009899258],"category_scores_gemma":[0.0006636145,0.00011886501,0.000069932095,0.00025779198,0.0003278311,0.00024074638,0.0006700414,0.00017679537,0.0001485277],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041353196,0.00008559862,0.71901953,0.00007969186,0.000095617004,0.0007789381,0.0012939943,0.0035905384,0.25324506,0.002824776,0.0003075708,0.018265212],"study_design_scores_gemma":[0.0000089299,0.000068045556,0.99443465,0.000004935163,0.0000104465735,0.00026568474,0.0002440903,0.0019394212,0.0022157824,0.00035429632,0.00044521198,0.0000085218235],"about_ca_topic_score_codex":0.0023345593,"about_ca_topic_score_gemma":0.0037364175,"teacher_disagreement_score":0.0023345593,"about_ca_system_score_codex":0.00024109437,"about_ca_system_score_gemma":0.000093381605,"threshold_uncertainty_score":0.0046418905},"labels":[],"label_agreement":null},{"id":"W2116893474","doi":"10.1088/0004-637x/766/2/88","title":"SPECTRAL PROPERTIES OF X-RAY BINARIES IN CENTAURUS A","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Spectral properties; Centaurus A; Stars; Stellar evolution; X-ray astronomy","score_opus":0.014481714672995598,"score_gpt":0.20610171294199145,"score_spread":0.19161999826899584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2116893474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99967504,0.000047633202,0.000024892797,0.0000044917524,0.0000012475955,0.000001442196,0.000069095375,0.0000043047485,0.00017182586],"genre_scores_gemma":[0.99964905,0.000021093161,0.0000422714,0.000005774496,0.0000038615076,0.0000017071819,0.00017803868,0.00000156469,0.000096635886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998325,0.000015517318,0.000022318553,0.00005290856,0.000029930705,0.00004685798],"domain_scores_gemma":[0.99893135,0.00012779619,0.00043075762,0.000071220384,0.00008275808,0.00035609855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002958891,0.00032524695,0.0002915073,0.0026166602,0.000538367,0.0008530189,0.0002715986,0.00027239812,0.0013384733],"category_scores_gemma":[0.00089687994,0.00017343099,0.00019422945,0.0010876568,0.00040654073,0.00048619192,0.00085571024,0.00023979704,0.00042853167],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016824222,0.000050461065,0.99166894,0.000007543077,0.000023436964,0.00012009908,0.00028712951,0.00007909983,0.004895318,0.000035641595,0.00006354401,0.0026004503],"study_design_scores_gemma":[0.0000018555374,0.000038918224,0.99920887,0.0000016176555,0.0000062371023,0.00015371917,0.00010858613,0.00013253203,0.00024611107,0.00002343362,0.00007529544,0.000002868409],"about_ca_topic_score_codex":0.0033841112,"about_ca_topic_score_gemma":0.00492505,"teacher_disagreement_score":0.0033841112,"about_ca_system_score_codex":0.00033174924,"about_ca_system_score_gemma":0.000099466466,"threshold_uncertainty_score":0.006728828},"labels":[],"label_agreement":null},{"id":"W2117482580","doi":"10.1088/0004-637x/753/2/144","title":"ANCHORING THE DISTANCE SCALE VIA X-RAY/INFRARED DATA FOR CEPHEID CLUSTERS: SU Cas","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Saint Mary's University","funders":"","keywords":"Cepheid variable; Physics; Astrophysics; Sky; Cluster (spacecraft); Proper motion; Star cluster; Stars; Astronomy; Computer science","score_opus":0.024247408950103026,"score_gpt":0.2578038376004367,"score_spread":0.23355642865033366,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2117482580","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897181,0.000064325075,0.00083635846,0.000045148627,0.0000133900585,0.00001946719,0.0011073358,0.00004874339,0.008147182],"genre_scores_gemma":[0.99711823,0.000020112018,0.001495019,0.000010298679,0.0000041400353,0.0000074609466,0.0009455351,0.000007870612,0.00039130016],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998386,0.000018928875,0.00001576056,0.000057126246,0.00004247449,0.000027136713],"domain_scores_gemma":[0.99879515,0.00013473777,0.00022634913,0.00029654906,0.00033866672,0.00020854447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038472717,0.00019707582,0.00018532184,0.0015385543,0.0006796217,0.00065884314,0.0003229007,0.00013190003,0.0015523444],"category_scores_gemma":[0.0021806683,0.000076969605,0.00009640862,0.001385158,0.0002538895,0.0003042267,0.0007284748,0.00029043152,0.0004091634],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027207533,0.00003671073,0.954073,0.00003547751,0.000029034763,0.00014933842,0.0007147151,0.0010235443,0.0069327187,0.001978925,0.0024209279,0.032333504],"study_design_scores_gemma":[0.000007879943,0.00002810874,0.992717,0.0000067849714,0.0000101414535,0.000060284518,0.00026854553,0.0020724721,0.0010218344,0.000349176,0.003451636,0.000006073419],"about_ca_topic_score_codex":0.035505097,"about_ca_topic_score_gemma":0.062420245,"teacher_disagreement_score":0.035505097,"about_ca_system_score_codex":0.00049004605,"about_ca_system_score_gemma":0.00038331698,"threshold_uncertainty_score":0.070596874},"labels":[],"label_agreement":null},{"id":"W2117575442","doi":"10.1086/524730","title":"The Rich Mid-Infrared Environments of Two Highly Obscured X-Ray Binaries: <i>Spitzer</i> Observations of IGR J16318-4848 and GX 301-2","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Extinction (optical mineralogy); Ionization; Silicate; Spectral line; Observable; Spectroscopy; Emission spectrum; Absorption (acoustics); H II region","score_opus":0.013368403810723432,"score_gpt":0.231481367731709,"score_spread":0.21811296392098556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2117575442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994246,0.00003858868,0.000049133727,0.000011982421,0.0000013440147,0.0000015900481,0.00007758823,0.0000075128514,0.0003877429],"genre_scores_gemma":[0.9994412,0.000025515961,0.00017352458,0.000019242154,0.00000762248,0.0000024989706,0.00023929247,0.000002986854,0.00008802431],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999126,0.000006007616,0.0000056995545,0.000026090644,0.000020540097,0.000029038427],"domain_scores_gemma":[0.9998287,0.000010879155,0.00008261106,0.000015484355,0.000011979505,0.00005033321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008840622,0.00016853926,0.00022915642,0.00065119035,0.00033425502,0.00047401246,0.00025052094,0.00027484956,0.0009778365],"category_scores_gemma":[0.00016714324,0.000105790205,0.00010741388,0.00031714878,0.00021501398,0.00031353516,0.000621021,0.00024050272,0.0003056256],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004951707,0.00018649934,0.80540764,0.000041523082,0.000066843895,0.0014639192,0.00050868286,0.00031657887,0.18263151,0.00023028693,0.00041911998,0.008232289],"study_design_scores_gemma":[0.00001571081,0.000045198853,0.9960877,0.0000036470267,0.000012020214,0.00066304044,0.00010168617,0.00029958942,0.0022208744,0.00006659292,0.0004793092,0.000004613317],"about_ca_topic_score_codex":0.0012205208,"about_ca_topic_score_gemma":0.003263712,"teacher_disagreement_score":0.0012205208,"about_ca_system_score_codex":0.0001963505,"about_ca_system_score_gemma":0.000075343276,"threshold_uncertainty_score":0.003271222},"labels":[],"label_agreement":null},{"id":"W2117686248","doi":"10.1086/378154","title":"The Unusual 2001 Periastron Passage in the “Clockwork” Colliding‐Wind Binary WR 140","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Université du Québec à Montréal; Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Photometry (optics); Orbital period; Orbital inclination; Emission spectrum; Astronomy; Orbital eccentricity; Orbital elements; Wolf–Rayet star; Ionization; Spectral line; Binary number; Stars","score_opus":0.013532536248833778,"score_gpt":0.2391887428201637,"score_spread":0.22565620657132993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2117686248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9782753,0.00014747232,0.0005773521,0.0009227214,0.00028921163,0.0000088798115,0.00014361883,0.00005347444,0.019582033],"genre_scores_gemma":[0.996396,0.000056662684,0.0002241012,0.00022922731,0.00006862622,0.000003535863,0.00022168306,0.000019011615,0.0027810591],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999356,0.000005434017,0.0000044983426,0.00002008081,0.000013319852,0.000020928546],"domain_scores_gemma":[0.9996494,0.00004992398,0.00010895107,0.000045772686,0.000043392625,0.00010254145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025888954,0.00013921224,0.00022941067,0.00047784997,0.002222879,0.0016052459,0.0003018366,0.0014838976,0.0026922568],"category_scores_gemma":[0.00120143,0.0001771352,0.0001595423,0.0005794844,0.00030753014,0.00061160105,0.0008600877,0.0013597155,0.0006067392],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0051661525,0.0008144965,0.3718692,0.00032215923,0.00030245882,0.12024163,0.009694673,0.0109316325,0.1725497,0.08612206,0.058268707,0.16371717],"study_design_scores_gemma":[0.00018212583,0.0010669813,0.83125496,0.00014300251,0.00011715486,0.028021421,0.004732697,0.008591386,0.010400546,0.013848282,0.10146112,0.00018034199],"about_ca_topic_score_codex":0.0033417966,"about_ca_topic_score_gemma":0.009275158,"teacher_disagreement_score":0.0033417966,"about_ca_system_score_codex":0.00061220734,"about_ca_system_score_gemma":0.00028176396,"threshold_uncertainty_score":0.0090065},"labels":[],"label_agreement":null},{"id":"W2117845751","doi":"10.1088/0004-637x/769/1/55","title":"<i>HERSCHEL</i>EXPLOITATION OF LOCAL GALAXY ANDROMEDA (HELGA). III. THE STAR FORMATION LAW IN M31","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; Star formation; Galaxy; Andromeda Galaxy; RADIUS; Andromeda; Spiral galaxy; Luminosity; Stars; Power law; Milky Way; Statistics","score_opus":0.009643847476539243,"score_gpt":0.22229768226517382,"score_spread":0.2126538347886346,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2117845751","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07208625,0.014455246,0.058342166,0.0052044876,0.00093775353,0.00031114052,0.3058663,0.06958332,0.47321337],"genre_scores_gemma":[0.49530265,0.007309731,0.13715555,0.0022233333,0.000676986,0.0004900118,0.24740212,0.012236401,0.09720327],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9998153,0.000035500292,0.000008372794,0.000040425122,0.00006445768,0.000035985486],"domain_scores_gemma":[0.999652,0.000029585914,0.00004527277,0.00016198182,0.00005100398,0.000060172213],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004996343,0.00051681435,0.0002426031,0.0015490014,0.0003086554,0.00087961834,0.00078250945,0.00029473082,0.03546548],"category_scores_gemma":[0.00073926465,0.00017298375,0.00027142128,0.0013428957,0.00021212794,0.00081381825,0.0012128345,0.0004048491,0.026528431],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025935227,0.00003515485,0.03745631,0.0004027598,0.00009367916,0.0002325006,0.00032236887,0.0015640055,0.0072215814,0.03929803,0.5808889,0.33222535],"study_design_scores_gemma":[0.000027868964,0.000019337913,0.04885594,0.00009043731,0.000008207991,0.000270995,0.00007087087,0.0013151455,0.002639123,0.0051875073,0.94148153,0.000033028122],"about_ca_topic_score_codex":0.0090269055,"about_ca_topic_score_gemma":0.012368229,"teacher_disagreement_score":0.03546548,"about_ca_system_score_codex":0.0005043352,"about_ca_system_score_gemma":0.00025951207,"threshold_uncertainty_score":0.11864382},"labels":[],"label_agreement":null},{"id":"W2117895447","doi":"10.1086/343068","title":"The Structure and Evolution of the Lagoon Nebula. I. Submillimeter Continuum and CO Line Mapping","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics; Saint Mary's University","funders":"","keywords":"Physics; Nebula; Protoplanetary nebula; Astronomy; Astrophysics; Line (geometry); Emission nebula; Astrobiology; Stars","score_opus":0.009062607806083832,"score_gpt":0.1969863319894606,"score_spread":0.18792372418337677,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2117895447","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99537563,0.0005089171,0.0003452801,0.000061559556,0.000003744086,0.0000043902523,0.0003264825,0.000043851585,0.0033301658],"genre_scores_gemma":[0.9984994,0.00013650027,0.000491602,0.000016682125,0.000004506251,0.0000033404012,0.00026927257,0.000008494683,0.0005702485],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999721,0.0000021502117,7.9519003e-7,0.000007797788,0.000005096144,0.00001193144],"domain_scores_gemma":[0.9998361,0.000020921414,0.000060368333,0.0000127501435,0.00002651235,0.000043497686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000062536004,0.00012287595,0.000064290725,0.00087168574,0.00021152102,0.0005051801,0.00024313803,0.00018312632,0.0011598892],"category_scores_gemma":[0.0003152385,0.00012531529,0.00005819878,0.0005872359,0.00021032985,0.0002396174,0.00032844837,0.00020600349,0.00030124583],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018464847,0.00004607292,0.8828805,0.000040535935,0.000018630291,0.000710083,0.0005455822,0.0021374878,0.06325815,0.0017371017,0.0008402534,0.047600843],"study_design_scores_gemma":[0.0000067163774,0.000024372606,0.9931851,0.00001195716,0.000004302829,0.00037076153,0.00012844142,0.0016595712,0.0011961625,0.00039378746,0.0030137154,0.000005126644],"about_ca_topic_score_codex":0.01445607,"about_ca_topic_score_gemma":0.016540436,"teacher_disagreement_score":0.01445607,"about_ca_system_score_codex":0.00052688393,"about_ca_system_score_gemma":0.00013222266,"threshold_uncertainty_score":0.028743863},"labels":[],"label_agreement":null},{"id":"W2118117006","doi":"10.1088/0004-637x/792/1/62","title":"BICEP2. II. EXPERIMENT AND THREE-YEAR DATA SET","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":226,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia","funders":"","keywords":"Cosmic microwave background; Physics; Transition edge sensor; Detector; Bolometer; Optics; Polarization (electrochemistry); Telescope; Gravitational wave; Cosmic background radiation; South Pole Telescope; Astrophysics","score_opus":0.01818651428709445,"score_gpt":0.2762195547047471,"score_spread":0.2580330404176526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118117006","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.42260453,0.0007899083,0.025831798,0.002780399,0.0004328398,0.0043282947,0.48889363,0.007881272,0.046457376],"genre_scores_gemma":[0.21225117,0.00029763478,0.06933408,0.0024188529,0.0002536433,0.008185059,0.6979706,0.0014334262,0.007855517],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9981652,0.00032322016,0.000084473075,0.00038714206,0.00062327686,0.00041675812],"domain_scores_gemma":[0.99545056,0.00045501668,0.00027335688,0.002007057,0.0011638799,0.00065012684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004072591,0.0012543334,0.0012374794,0.0017942351,0.0033671902,0.001723435,0.0033090867,0.0017567055,0.0076705986],"category_scores_gemma":[0.002410417,0.0007854204,0.00081445783,0.0032177027,0.0010611746,0.001582886,0.0037383032,0.002404702,0.0069570853],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.009782289,0.0057984875,0.15128604,0.0015857853,0.0011694487,0.0047389558,0.0012669018,0.018100034,0.07282298,0.020321812,0.59834826,0.11477897],"study_design_scores_gemma":[0.004590696,0.0020750244,0.3173064,0.00024191325,0.00033379986,0.0033448003,0.0009814788,0.029923173,0.051213894,0.00996651,0.5793723,0.0006499452],"about_ca_topic_score_codex":0.014650452,"about_ca_topic_score_gemma":0.020554597,"teacher_disagreement_score":0.014650452,"about_ca_system_score_codex":0.001114976,"about_ca_system_score_gemma":0.001975149,"threshold_uncertainty_score":0.0291304},"labels":[],"label_agreement":null},{"id":"W2118139755","doi":"10.1088/0004-637x/775/1/48","title":"CONTINUED NEUTRON STAR CRUST COOLING OF THE 11 Hz X-RAY PULSAR IN TERZAN 5: A CHALLENGE TO HEATING AND COOLING MODELS?","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution","keywords":"Neutron star; Pulsar; Globular cluster; Crust; Accretion (finance); X-ray pulsar; X-ray binary; Flux (metallurgy)","score_opus":0.017335197759771503,"score_gpt":0.22753127653544966,"score_spread":0.21019607877567817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118139755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974904,0.0007029946,0.00033075447,0.00026284528,0.000017282528,0.000003681646,0.00005382072,0.000018924515,0.0011192928],"genre_scores_gemma":[0.9992817,0.00025022775,0.00013914912,0.000056678433,0.000012142537,0.0000021042613,0.0000771159,0.0000074502286,0.00017342706],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999075,0.0000117427335,0.000007018148,0.000032435375,0.000011279068,0.000030014644],"domain_scores_gemma":[0.9998061,0.000024632922,0.00007792038,0.00003634716,0.000021981868,0.000033064436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044746918,0.00032911633,0.00064723537,0.00032629017,0.00068691437,0.001045618,0.00067480956,0.00060051493,0.00094158505],"category_scores_gemma":[0.0005929255,0.00027178795,0.00036812678,0.00022643156,0.0009350521,0.0011288417,0.00071713567,0.00065829046,0.0002161682],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010415815,0.00012592187,0.8116625,0.00024599792,0.00027767415,0.0018110118,0.0015542551,0.00788342,0.14768952,0.005043452,0.0006693641,0.021995328],"study_design_scores_gemma":[0.000043429074,0.00019028886,0.9747624,0.000044750264,0.00006353844,0.0006929573,0.0011447468,0.012666546,0.0051923255,0.0026753403,0.0024921936,0.000031516807],"about_ca_topic_score_codex":0.004422947,"about_ca_topic_score_gemma":0.004496879,"teacher_disagreement_score":0.004422947,"about_ca_system_score_codex":0.0008377874,"about_ca_system_score_gemma":0.0002906088,"threshold_uncertainty_score":0.008794367},"labels":[],"label_agreement":null},{"id":"W2118272902","doi":"10.1088/0004-637x/769/1/33","title":"<i>MOST</i>OBSERVATIONS OF σ Ori E: CHALLENGING THE CENTRIFUGAL BREAKOUT NARRATIVE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto; St. Mary's University; University of British Columbia; Saint Mary's University; Université de Montréal","funders":"","keywords":"Breakout; Physics; Astrophysics; Magnetosphere; Astronomy; Plasma; Eclipse; Nuclear physics","score_opus":0.015075991241891528,"score_gpt":0.22004608278622637,"score_spread":0.20497009154433485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118272902","genre_codex":"commentary","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0060961014,0.024917306,0.0037193657,0.8072739,0.06932078,0.000025415082,0.0008417402,0.00035708872,0.08744821],"genre_scores_gemma":[0.1583579,0.030835927,0.0036972137,0.32933605,0.40352696,0.00007012811,0.001431192,0.0007687709,0.07197589],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99923944,0.00011824541,0.000040796884,0.00017255757,0.00026938168,0.00015973204],"domain_scores_gemma":[0.99449015,0.0018526128,0.00061947736,0.0005222206,0.001649756,0.0008657595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004180586,0.00058905047,0.00046490543,0.0017776366,0.0033539059,0.0070884773,0.001797177,0.0058974586,0.01577058],"category_scores_gemma":[0.010402285,0.00019337461,0.00040366658,0.001665894,0.0034727198,0.00742813,0.0044042864,0.006079487,0.004633708],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007098506,0.000015133002,0.0024661978,0.00030111172,0.000022653463,0.00028527153,0.000851549,0.00011499113,0.0023268822,0.028523337,0.9119202,0.053101722],"study_design_scores_gemma":[0.000008844871,0.000020842352,0.006078314,0.00033847886,0.000016605614,0.000324608,0.0019094078,0.00010657436,0.00086752785,0.03354048,0.9567581,0.000030316884],"about_ca_topic_score_codex":0.0028501549,"about_ca_topic_score_gemma":0.0064879283,"teacher_disagreement_score":0.01577058,"about_ca_system_score_codex":0.0012018558,"about_ca_system_score_gemma":0.0012091346,"threshold_uncertainty_score":0.05275786},"labels":[],"label_agreement":null},{"id":"W2118463792","doi":"10.1088/0004-637x/773/2/170","title":"A MULTIPLICITY CENSUS OF INTERMEDIATE-MASS STARS IN SCORPIUS-CENTAURUS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal","funders":"","keywords":"Physics; Stars; Astrophysics; Multiplicity (mathematics); Astronomy; Brown dwarf; Stellar mass; Star formation","score_opus":0.01072665640738969,"score_gpt":0.2234245734936327,"score_spread":0.21269791708624303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118463792","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993049,0.00007859199,0.00006526705,0.0000043944083,6.2958367e-7,0.0000017692527,0.00013539159,0.0000107253045,0.00039833688],"genre_scores_gemma":[0.9988636,0.00009568726,0.00021248225,0.00000411276,0.0000029088867,0.0000031962925,0.0006049949,0.0000048808247,0.00020827711],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998828,0.00000632731,0.000008790684,0.00004566642,0.000021430707,0.000034899018],"domain_scores_gemma":[0.9995291,0.00004182346,0.0001570088,0.00003645754,0.00005689672,0.00017855612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014736065,0.00019606594,0.00023239283,0.0027212726,0.00044259574,0.00063517824,0.0001909777,0.00018878485,0.0012529208],"category_scores_gemma":[0.00056543516,0.00014594062,0.0001392761,0.0011085955,0.00046713854,0.00034139754,0.0008853961,0.00014069863,0.00035463882],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006866506,0.000008173754,0.9822432,0.00001671941,0.000011817547,0.00015233443,0.00038156204,0.00006202448,0.00953962,0.00007577788,0.00007426276,0.0073658573],"study_design_scores_gemma":[7.385581e-7,0.00001830879,0.99875104,0.0000025680674,0.000004308446,0.00024936965,0.00013400639,0.00006126852,0.00050625525,0.000024751982,0.0002457141,0.0000016727506],"about_ca_topic_score_codex":0.0044932324,"about_ca_topic_score_gemma":0.0065804357,"teacher_disagreement_score":0.0044932324,"about_ca_system_score_codex":0.00029929998,"about_ca_system_score_gemma":0.00020262245,"threshold_uncertainty_score":0.00893414},"labels":[],"label_agreement":null},{"id":"W2118618078","doi":"10.1088/0004-637x/799/2/242","title":"ERRATUM: “THREE-DIMENSIONAL ATMOSPHERIC CIRCULATION MODELS OF HD 189733b AND HD 209458b WITH CONSISTENT MAGNETIC DRAG AND OHMIC DISSIPATION” (2013, ApJ, 764, 103)","year":2015,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Geophysics and Gravity Measurements","field":"Earth and Planetary Sciences","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"","keywords":"Physics; Drag; Astrophysics; Circulation (fluid dynamics); Eddy current brake; Astronomy; Mechanics; Magnetic field","score_opus":0.019198563638185118,"score_gpt":0.19857914971765292,"score_spread":0.1793805860794678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118618078","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0017639039,0.00057815557,0.001030687,0.029919831,0.93275917,0.000053106876,0.017038397,0.0009878537,0.01586899],"genre_scores_gemma":[0.05850105,0.0029076936,0.01068602,0.051847987,0.11960499,0.00029018155,0.07469541,0.0050533754,0.6764132],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99905175,0.000073353694,0.00019350208,0.00015031447,0.0004349674,0.00009610149],"domain_scores_gemma":[0.99489117,0.00073646515,0.0003744836,0.00048325426,0.0031917102,0.00032296873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011020651,0.0016122926,0.0011849124,0.0020887852,0.0033541673,0.0026299537,0.0020722363,0.0027162086,0.070199125],"category_scores_gemma":[0.013330898,0.00088610203,0.0012474088,0.0015689558,0.0010886674,0.0023233546,0.0015705101,0.004062884,0.033474285],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004285219,0.000009260041,0.00019173452,0.000029504505,0.000007876529,0.000099995385,0.000013820033,0.00010745612,0.000076776974,0.00050088007,0.9970155,0.0019044419],"study_design_scores_gemma":[0.00013729424,0.000041441144,0.008169407,0.00018449887,0.0000599059,0.000233031,0.00019396594,0.0010104538,0.0010153314,0.002566182,0.9863166,0.00007178151],"about_ca_topic_score_codex":0.04662698,"about_ca_topic_score_gemma":0.07044743,"teacher_disagreement_score":0.070199125,"about_ca_system_score_codex":0.0032804906,"about_ca_system_score_gemma":0.0040157423,"threshold_uncertainty_score":0.2348395},"labels":[],"label_agreement":null},{"id":"W2118661612","doi":"10.1088/0004-637x/768/1/9","title":"THE Q/U IMAGING EXPERIMENT INSTRUMENT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Fermilab; Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Kavli Institute for Cosmological Physics, University of Chicago; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; Northrop Grumman; Jet Propulsion Laboratory; Alfred P. Sloan Foundation; Universitetet i Oslo","keywords":"Polarimeter; Physics; Cosmic microwave background; Sensitivity (control systems); Gravitational wave; Telescope; Optics; High-electron-mobility transistor; Polarization (electrochemistry); Calibration; Stokes parameters; Polarimetry; Microwave; Astrophysics; Transistor; Electronic engineering; Anisotropy; Engineering","score_opus":0.007044973024672309,"score_gpt":0.21475334575303467,"score_spread":0.20770837272836237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118661612","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.15823899,0.0010453628,0.10753944,0.0035793711,0.0012447629,0.0044486155,0.19041178,0.037192184,0.49629956],"genre_scores_gemma":[0.44692925,0.0007413612,0.26656875,0.003756371,0.00085042795,0.004177977,0.16994947,0.0054438785,0.10158254],"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9989158,0.00013453959,0.000036910318,0.00037336806,0.00035669646,0.00018271367],"domain_scores_gemma":[0.99895144,0.000069164984,0.00010954208,0.00032664978,0.00037550504,0.00016763766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00200614,0.00042000052,0.00035877698,0.000843838,0.0009941217,0.00095638545,0.0009552417,0.00062142895,0.027492],"category_scores_gemma":[0.0013282279,0.00037171395,0.00023972664,0.000824439,0.00046187392,0.0010886805,0.0013303173,0.00085409934,0.01768721],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025544772,0.0005047387,0.030388743,0.0002688875,0.00007928997,0.00027156348,0.00034118257,0.0018371507,0.099964134,0.034364734,0.6723352,0.15708989],"study_design_scores_gemma":[0.000721905,0.00050533866,0.042481698,0.00008141049,0.00006151372,0.00025269712,0.00012342048,0.009469603,0.03549402,0.0048720823,0.9058203,0.00011593374],"about_ca_topic_score_codex":0.0043321047,"about_ca_topic_score_gemma":0.005898191,"teacher_disagreement_score":0.027492,"about_ca_system_score_codex":0.0008010696,"about_ca_system_score_gemma":0.0016334535,"threshold_uncertainty_score":0.09196985},"labels":[],"label_agreement":null},{"id":"W2118836848","doi":"10.1088/0004-637x/731/1/31","title":"EVIDENCE FOR RAPID REDSHIFT EVOLUTION OF STRONG CLUSTER COOLING FLOWS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Redshift; Luminosity; Cluster (spacecraft); Galaxy; Emission spectrum; Galaxy cluster; Galaxy groups and clusters; Cooling flow","score_opus":0.03371052848621807,"score_gpt":0.2488969766939398,"score_spread":0.2151864482077217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2118836848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993944,0.00009013924,0.0000538997,0.000012577308,0.0000010318265,0.0000019596039,0.000049072958,0.0000072095886,0.00038971362],"genre_scores_gemma":[0.99972004,0.00003027116,0.00006352618,0.0000059687995,0.000003531749,0.0000010762529,0.000071955365,0.0000014680194,0.000102116464],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985874,0.000011839844,0.000006554416,0.000043286425,0.000023942564,0.000055544144],"domain_scores_gemma":[0.9987263,0.00022782976,0.0004661572,0.000120851626,0.00013645539,0.00032239826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027919523,0.0001886429,0.00018133681,0.00076108245,0.00031305215,0.00052186433,0.00025175934,0.0002509431,0.0017370436],"category_scores_gemma":[0.0009938797,0.00019732288,0.000120603865,0.00030821405,0.00047780783,0.00026979946,0.0005906902,0.0002568132,0.00016980035],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017211394,0.00003561816,0.9696269,0.000023601286,0.000038316193,0.00025067065,0.00026575566,0.00031107815,0.023255251,0.00052036403,0.00011534671,0.005385077],"study_design_scores_gemma":[0.000004421424,0.00002155236,0.99880624,0.00000156698,0.0000056532112,0.00015137589,0.000029373583,0.00015269937,0.0006173227,0.000046239034,0.00016090905,0.0000026627586],"about_ca_topic_score_codex":0.0035585875,"about_ca_topic_score_gemma":0.004935018,"teacher_disagreement_score":0.0035585875,"about_ca_system_score_codex":0.00031984178,"about_ca_system_score_gemma":0.0001947433,"threshold_uncertainty_score":0.007075727},"labels":[],"label_agreement":null},{"id":"W2119510649","doi":"10.1088/0004-637x/725/2/1587","title":"<i>z</i>∼ 7 GALAXY CANDIDATES FROM NICMOS OBSERVATIONS OVER THE HDF-SOUTH AND THE CDF-SOUTH AND HDF-NORTH GOODS FIELDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Galaxy; Astrophysics; Supernova; Star formation; Stars; Galaxy formation and evolution","score_opus":0.007425606078463148,"score_gpt":0.1956772902551975,"score_spread":0.18825168417673435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119510649","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937953,0.0000842055,0.0006951819,0.000032387055,0.000002669871,0.000043826993,0.0016279853,0.00010657737,0.0036117882],"genre_scores_gemma":[0.9758704,0.00016372546,0.005670793,0.00005891497,0.0000113939805,0.00009576543,0.01600167,0.000047904618,0.0020794135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998171,0.000017170552,0.000011715375,0.00003562693,0.000058798963,0.00005972064],"domain_scores_gemma":[0.9995937,0.00007498843,0.0001152616,0.000064194915,0.00006459316,0.000087358705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033623722,0.00018607579,0.00021335372,0.0012598502,0.00046597622,0.0006235654,0.00043562808,0.00018326084,0.0028321284],"category_scores_gemma":[0.0006975965,0.00012374265,0.00035621307,0.0010335634,0.0001354819,0.00014333351,0.0006455324,0.00014142928,0.00070346874],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003822464,0.00012326491,0.9246453,0.0001261546,0.00013667194,0.0013902386,0.0006854888,0.0064176912,0.016307477,0.0032221973,0.0072417525,0.03932151],"study_design_scores_gemma":[0.000054097385,0.00012446831,0.94994885,0.00004889609,0.00012356615,0.0010220276,0.0005358015,0.017667536,0.0108833965,0.0009469922,0.018612511,0.00003193908],"about_ca_topic_score_codex":0.008281237,"about_ca_topic_score_gemma":0.02804749,"teacher_disagreement_score":0.008281237,"about_ca_system_score_codex":0.00042369042,"about_ca_system_score_gemma":0.00045717997,"threshold_uncertainty_score":0.016466081},"labels":[],"label_agreement":null},{"id":"W2119611011","doi":"10.1086/324694","title":"<i>Far Ultraviolet Spectroscopic Explorer</i>Observations of the Seyfert 1.5 Galaxy NGC 5548 in a Low State","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Galaxy; Astrophysics; Ultraviolet; Ionization; Spectral line; Emission spectrum; Far ultraviolet; Active galactic nucleus; Absorption (acoustics); Absorption spectroscopy; Wavelength; Astronomy; Optics; Ion","score_opus":0.013918784699161411,"score_gpt":0.20649881082368354,"score_spread":0.19258002612452213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119611011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99826497,0.00009794879,0.00009955627,0.000020416042,0.0000035903427,0.0000021906108,0.00046280888,0.000034386343,0.0010141258],"genre_scores_gemma":[0.99796045,0.00006365571,0.0003775404,0.000016379208,0.00001281683,0.0000031562886,0.0011902947,0.00000541598,0.00037016536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999267,0.0000054153447,0.000004579165,0.000021811626,0.00002010631,0.000021466403],"domain_scores_gemma":[0.9997937,0.000018448483,0.00008500802,0.000027629188,0.00002187313,0.00005333269],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011808573,0.00021904884,0.00019090288,0.0010984705,0.00032482488,0.00036769838,0.00022803983,0.00024536738,0.0014268755],"category_scores_gemma":[0.00025795156,0.00010292168,0.00019079662,0.0003874726,0.00015593016,0.00025258932,0.00030411244,0.00021725547,0.00024881182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005674484,0.00019049937,0.87077945,0.00006617758,0.00019657816,0.0014463736,0.00065585383,0.0013449504,0.10388015,0.00031494527,0.0020044737,0.018553134],"study_design_scores_gemma":[0.000008812448,0.000063623105,0.9968387,0.000005568913,0.000019129717,0.00029443414,0.000056179324,0.00033871908,0.0014162373,0.000043692624,0.0009096352,0.0000052717814],"about_ca_topic_score_codex":0.0040384494,"about_ca_topic_score_gemma":0.010429228,"teacher_disagreement_score":0.0040384494,"about_ca_system_score_codex":0.00022925541,"about_ca_system_score_gemma":0.00005211403,"threshold_uncertainty_score":0.008029878},"labels":[],"label_agreement":null},{"id":"W2119653766","doi":"10.1088/0004-637x/723/1/915","title":"THE BLAST VIEW OF THE STAR-FORMING REGION IN AQUILA (ℓ = 45°,<i>b</i>= 0°)","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of British Columbia; University of Toronto","funders":"","keywords":"Stars; Population; Stellar population; Stellar evolution; Star formation; Emissivity; Bolometer; Range (aeronautics)","score_opus":0.00864995120325432,"score_gpt":0.2300673763425339,"score_spread":0.2214174251392796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119653766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94610023,0.00013618228,0.00083885994,0.00031025597,0.000024278237,0.000042677715,0.0049957894,0.00022981782,0.04732202],"genre_scores_gemma":[0.98741406,0.000107819826,0.0026652983,0.00006413305,0.000022646953,0.000033005595,0.0027586822,0.000032927874,0.00690141],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995005,0.0000043540977,0.0000012793615,0.000014069575,0.000012717168,0.000017482473],"domain_scores_gemma":[0.9999194,0.0000062540207,0.000019688,0.000007323023,0.000015992557,0.000031337633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007290041,0.00017016227,0.00010519057,0.0007676592,0.0005958442,0.0003051397,0.00022938968,0.00013243401,0.008265881],"category_scores_gemma":[0.0001333975,0.0001735847,0.000098281984,0.0005813966,0.00033998015,0.00024142377,0.00063268957,0.00025242392,0.0013762226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014413794,0.00026645046,0.6875454,0.00026015766,0.00008367317,0.00328587,0.005286934,0.015527311,0.124591336,0.0072015934,0.037156973,0.11735292],"study_design_scores_gemma":[0.000046087487,0.000121689365,0.9667031,0.00004156857,0.000013612344,0.0004622683,0.00072604814,0.003095571,0.0020788352,0.00039293087,0.026300294,0.000018058501],"about_ca_topic_score_codex":0.038624164,"about_ca_topic_score_gemma":0.06106965,"teacher_disagreement_score":0.038624164,"about_ca_system_score_codex":0.00045527253,"about_ca_system_score_gemma":0.00047994047,"threshold_uncertainty_score":0.07679868},"labels":[],"label_agreement":null},{"id":"W2119792136","doi":"10.1088/0004-637x/772/1/15","title":"LACERTA I AND CASSIOPEIA III. TWO LUMINOUS AND DISTANT ANDROMEDA SATELLITE DWARF GALAXIES FOUND IN THE 3π PAN-STARRS1 SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Centre National de la Recherche Scientifique; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Andromeda; Physics; Local Group; Astrophysics; Dwarf galaxy; Galaxy; Dwarf spheroidal galaxy; Andromeda Galaxy; Astronomy; Surface brightness; Milky Way; Interacting galaxy","score_opus":0.016027607465960075,"score_gpt":0.2381165223758139,"score_spread":0.22208891490985383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119792136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879628,0.0008599836,0.0003572968,0.000052044496,0.000010132019,0.000024964102,0.0021898933,0.00015594071,0.008386949],"genre_scores_gemma":[0.9878905,0.00040962262,0.0011610662,0.0000663185,0.000029634813,0.000017664763,0.0068287663,0.000022820435,0.0035736237],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997569,0.0000077422155,0.000009009315,0.00009850579,0.00006397002,0.00006385391],"domain_scores_gemma":[0.9995334,0.000018375069,0.00022799821,0.000047415313,0.000034649678,0.0001382266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014960112,0.00055087486,0.00025222087,0.00090368435,0.00044838802,0.0007642006,0.0002779867,0.00017874346,0.0022420732],"category_scores_gemma":[0.00029994044,0.00013085012,0.00030848596,0.0008154895,0.00027490957,0.00021934102,0.0006459542,0.00026052303,0.00062546413],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042734572,0.000056678717,0.9205377,0.00010812501,0.0001780069,0.0008175551,0.00064134604,0.00026671204,0.03982513,0.0010734535,0.0021687911,0.033899162],"study_design_scores_gemma":[0.000013882073,0.00008527271,0.9864095,0.0000104717465,0.000046361612,0.0007743076,0.00015621803,0.000115879666,0.0025258604,0.00010022431,0.009753213,0.000008672198],"about_ca_topic_score_codex":0.011085059,"about_ca_topic_score_gemma":0.020535398,"teacher_disagreement_score":0.011085059,"about_ca_system_score_codex":0.00047568264,"about_ca_system_score_gemma":0.00024964707,"threshold_uncertainty_score":0.022041082},"labels":[],"label_agreement":null},{"id":"W2119850695","doi":"10.1088/0004-637x/784/2/148","title":"SPATIALLY RESOLVED IMAGING OF THE TWO-COMPONENT η Crv DEBRIS DISK WITH<i>HERSCHEL</i>","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Debris; Radiative transfer; Debris disk; Population; Asteroid belt; Astronomy; Brightness; Solar System; Planet; Planetary system; Optics","score_opus":0.005848575675661162,"score_gpt":0.21376766278573445,"score_spread":0.2079190871100733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119850695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8920967,0.0014981625,0.009851568,0.004107683,0.00013572174,0.000101356134,0.015650557,0.0021474382,0.074410826],"genre_scores_gemma":[0.9636263,0.0005886084,0.020237675,0.0010944153,0.00012709644,0.000047266272,0.0053516207,0.0002828632,0.008644168],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99984455,0.000014687294,0.000004653334,0.000045126468,0.000044348704,0.000046593315],"domain_scores_gemma":[0.99973625,0.00005149018,0.00004338758,0.000059561055,0.0000494194,0.00005982742],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044698658,0.00022116635,0.00020182112,0.00072120223,0.00044710847,0.00066865864,0.00041010897,0.00063439563,0.004937964],"category_scores_gemma":[0.0004082137,0.0003284111,0.000260025,0.00048562154,0.0002704178,0.00054803246,0.0005094058,0.0008043396,0.0008763666],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079777424,0.00024080854,0.036810745,0.0002513957,0.00025193547,0.0010533839,0.00033696022,0.0061102323,0.89262563,0.004591489,0.0256405,0.031289224],"study_design_scores_gemma":[0.00042084997,0.00039279225,0.7848875,0.00017129233,0.00021142581,0.0028405408,0.00051738136,0.02304093,0.12869899,0.004232577,0.05443412,0.00015159602],"about_ca_topic_score_codex":0.0040854476,"about_ca_topic_score_gemma":0.012739591,"teacher_disagreement_score":0.004937964,"about_ca_system_score_codex":0.00068852305,"about_ca_system_score_gemma":0.000558217,"threshold_uncertainty_score":0.016519189},"labels":[],"label_agreement":null},{"id":"W2119852497","doi":"10.1086/591026","title":"First Stellar Velocity Dispersion Measurement of a Luminous Quasar Host with Gemini North Laser Guide Star Adaptive Optics","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Laser guide star; Velocity dispersion; Galaxy; Luminosity; Adaptive optics; Supermassive black hole; Active galactic nucleus","score_opus":0.014719226431546575,"score_gpt":0.19320994445191073,"score_spread":0.17849071802036415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119852497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940164,0.00016018507,0.0039409357,0.000023330018,0.000008352223,0.000011912932,0.00014203419,0.00013702361,0.0015597253],"genre_scores_gemma":[0.9913658,0.00005040688,0.0076975753,0.00002441789,0.000011429906,0.0000057923394,0.00032580792,0.000011391917,0.0005072953],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998857,0.000010147566,0.000005013655,0.00003599392,0.000046096935,0.000017029002],"domain_scores_gemma":[0.9997191,0.000027862085,0.00007311031,0.000035675184,0.00008151348,0.00006279099],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025720376,0.00015547007,0.00012824424,0.0006080919,0.00033017792,0.00028617444,0.00031422908,0.00025938096,0.00047314476],"category_scores_gemma":[0.00025683056,0.00014641635,0.00009632977,0.00032008826,0.00017464971,0.00024774752,0.0003282427,0.00019691767,0.00014176534],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020263945,0.000085165506,0.60286325,0.00004354967,0.000078532925,0.00024869517,0.000442146,0.0005322479,0.35325667,0.000379574,0.0005249838,0.0413425],"study_design_scores_gemma":[0.000016032649,0.000454428,0.9405002,0.000007364907,0.000048750637,0.0005986628,0.00011131199,0.0027692004,0.051504012,0.000084076884,0.003888937,0.000016965567],"about_ca_topic_score_codex":0.001964811,"about_ca_topic_score_gemma":0.0057982835,"teacher_disagreement_score":0.001964811,"about_ca_system_score_codex":0.00024982827,"about_ca_system_score_gemma":0.0001032886,"threshold_uncertainty_score":0.003906727},"labels":[],"label_agreement":null},{"id":"W2119983994","doi":"10.1088/0004-637x/690/2/1208","title":"THE 5.25 AND 5.7 μm ASTRONOMICAL POLYCYCLIC AROMATIC HYDROCARBON EMISSION FEATURES","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Overtone; Physics; Spectral line; Spectrograph; Polycyclic aromatic hydrocarbon; Astrophysics; Population; Infrared spectroscopy; Full width at half maximum; Emission spectrum; Infrared; Astronomy; Optics","score_opus":0.007250323018850294,"score_gpt":0.21876559746290256,"score_spread":0.21151527444405227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119983994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98824394,0.00068597717,0.004395272,0.000043916665,0.000011972235,0.000011726169,0.00038120145,0.00016743361,0.0060585407],"genre_scores_gemma":[0.9957684,0.00011203669,0.0028445467,0.000031747364,0.000009666445,0.000008702884,0.00031603768,0.000011863688,0.0008968968],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999368,0.0000030224337,0.0000016351148,0.00002813042,0.000018824876,0.00001155684],"domain_scores_gemma":[0.99985766,0.000023877803,0.000057043664,0.000014010702,0.00002240382,0.000024970348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007951142,0.00017981167,0.00011251377,0.0005563471,0.0002565408,0.0002897155,0.00026869154,0.00027904302,0.002113709],"category_scores_gemma":[0.00016628817,0.00012299235,0.00021059472,0.0002681669,0.00024706533,0.00024855384,0.00018477504,0.00019048977,0.0003884316],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019239282,0.000091637536,0.17484541,0.00011679469,0.00006997961,0.0003871726,0.00021534567,0.00069552433,0.7680014,0.0018363278,0.0006509453,0.05289716],"study_design_scores_gemma":[0.000008998718,0.00021771231,0.8993131,0.00001086992,0.000038768776,0.0006405631,0.00013129212,0.0013886633,0.09147021,0.00069324824,0.0060725166,0.000014024339],"about_ca_topic_score_codex":0.00059511344,"about_ca_topic_score_gemma":0.0009180781,"teacher_disagreement_score":0.002113709,"about_ca_system_score_codex":0.0003083913,"about_ca_system_score_gemma":0.00007648582,"threshold_uncertainty_score":0.007071018},"labels":[],"label_agreement":null},{"id":"W2119984079","doi":"10.1088/0004-637x/769/2/130","title":"DISCOVERY OF A COSMOLOGICAL, RELATIVISTIC OUTBURST VIA ITS RAPIDLY FADING OPTICAL EMISSION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; Office of Science; Weizmann Institute of Science; University of Oxford; University of Leicester; Harvard University; W. M. Keck Foundation; Space Telescope Science Institute; Smithsonian Astrophysical Observatory; Massachusetts Institute of Technology; Gordon and Betty Moore Foundation; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution; Israel Science Foundation; James S. McDonnell Foundation; National Science Foundation","keywords":"Afterglow; Gamma-ray burst; Fading; Light curve; Transient (computer programming); Light emission","score_opus":0.01400954721067241,"score_gpt":0.23451281257460302,"score_spread":0.2205032653639306,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2119984079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975815,0.00020454774,0.0010434471,0.000049267383,0.000010247245,0.0000085216925,0.000096686956,0.000044815188,0.00096097804],"genre_scores_gemma":[0.99846625,0.00012879465,0.0007583498,0.000034294757,0.000025196203,0.000004870125,0.00027135634,0.0000065603854,0.00030436818],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999311,0.0000056490303,0.0000031274656,0.000033395252,0.000008676997,0.000018076482],"domain_scores_gemma":[0.99946374,0.00007831394,0.00021836392,0.00009277475,0.000033720204,0.000113067355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017099698,0.00025861867,0.00020565552,0.00049916666,0.0003749793,0.0006599281,0.0002795836,0.00029098056,0.0012370375],"category_scores_gemma":[0.0004233864,0.00017488385,0.0002037123,0.00026932018,0.00033171824,0.00025436294,0.00046107595,0.0003518243,0.00026068033],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005968344,0.00012899167,0.87063336,0.00011771064,0.00009420076,0.013324671,0.000821229,0.0003709609,0.07105044,0.0019056606,0.00088288885,0.040072985],"study_design_scores_gemma":[0.000046640766,0.00073318894,0.9468643,0.000027632843,0.00013019543,0.028555904,0.00037660456,0.001391522,0.011553988,0.000981004,0.009305026,0.00003392117],"about_ca_topic_score_codex":0.00068989553,"about_ca_topic_score_gemma":0.0005772741,"teacher_disagreement_score":0.0012370375,"about_ca_system_score_codex":0.0002219484,"about_ca_system_score_gemma":0.00012641055,"threshold_uncertainty_score":0.004138291},"labels":[],"label_agreement":null},{"id":"W2120006354","doi":"10.1088/0004-637x/787/1/9","title":"CONSTRAINING THE Lyα ESCAPE FRACTION WITH FAR-INFRARED OBSERVATIONS OF Lyα EMITTERS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Redshift; Galaxy; Infrared; Star formation; Astronomy; Far infrared; Flux (metallurgy)","score_opus":0.011409530169777084,"score_gpt":0.20558882219645877,"score_spread":0.1941792920266817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120006354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9876801,0.0008705748,0.005134565,0.000072230716,0.000008241721,0.000014249654,0.0005822395,0.000076971955,0.0055608447],"genre_scores_gemma":[0.9926501,0.00025972442,0.004679427,0.00004192991,0.00001615497,0.000011619355,0.0013125447,0.000025420717,0.0010031606],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996056,0.00007241604,0.000018182756,0.00015930003,0.00006979155,0.00007464598],"domain_scores_gemma":[0.99876344,0.0002786949,0.00031803077,0.00025235876,0.00021209818,0.00017542805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00090145966,0.0002993057,0.00025873064,0.0017930553,0.00037853667,0.0012650249,0.00046081384,0.00052736705,0.0012897188],"category_scores_gemma":[0.0022409416,0.00028540118,0.00027077357,0.0011313909,0.0002680938,0.0006470374,0.00085351727,0.0002905146,0.00061300345],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018618004,0.0000860134,0.92928034,0.000045062105,0.00011224095,0.00004925735,0.00020492465,0.0015665446,0.029494176,0.00064402696,0.00045419432,0.037877038],"study_design_scores_gemma":[0.000019373449,0.00004722734,0.9790299,0.000035080182,0.00007928953,0.00012737393,0.00034557204,0.009108745,0.004705709,0.0009066927,0.0055776807,0.000017421353],"about_ca_topic_score_codex":0.008653663,"about_ca_topic_score_gemma":0.019133337,"teacher_disagreement_score":0.008653663,"about_ca_system_score_codex":0.00036581734,"about_ca_system_score_gemma":0.0003011413,"threshold_uncertainty_score":0.01720661},"labels":[],"label_agreement":null},{"id":"W2120069867","doi":"10.1088/0004-637x/762/2/108","title":"THE COMPLEX PHYSICS OF DUSTY STAR-FORMING GALAXIES AT HIGH REDSHIFTS AS REVEALED BY<i>HERSCHEL</i>AND<i>SPITZER</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Star formation; Redshift; Photometry (optics); Stars; Luminous infrared galaxy; Spectral energy distribution; Stellar mass; Extinction (optical mineralogy); Infrared; Astronomy","score_opus":0.010763566974002655,"score_gpt":0.21947008961752373,"score_spread":0.20870652264352108,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120069867","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987557,0.00017183406,0.0006246307,0.000039371775,6.3356356e-7,0.0000027512503,0.000106678934,0.0000174779,0.00028100234],"genre_scores_gemma":[0.9992512,0.00009619789,0.00042687843,0.0000129604105,0.0000054902175,0.0000017551437,0.00014322306,0.0000025852903,0.000059695776],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977714,0.000055149303,0.000012908797,0.00006583075,0.000054780536,0.000034225057],"domain_scores_gemma":[0.99853253,0.00043463832,0.00071709545,0.00014347197,0.000043823504,0.00012843045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053592585,0.0002198649,0.000281696,0.0014293628,0.00028703656,0.0011289454,0.00052624405,0.00039431447,0.000674327],"category_scores_gemma":[0.0013006886,0.00029282458,0.00024467983,0.0011700307,0.0007571876,0.0011750209,0.00055492326,0.00025915084,0.00016359569],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024240835,0.000021958913,0.9879125,0.00001762032,0.00004673132,0.00011300015,0.00024250698,0.0018277355,0.006229051,0.00077100977,0.000051981333,0.0027417773],"study_design_scores_gemma":[0.000002318901,0.000018187788,0.99646676,0.000002191151,0.000010285876,0.000141252,0.00008874564,0.002044134,0.0004061822,0.0006336664,0.00018213886,0.000004179243],"about_ca_topic_score_codex":0.003517763,"about_ca_topic_score_gemma":0.0059883315,"teacher_disagreement_score":0.003517763,"about_ca_system_score_codex":0.0005340656,"about_ca_system_score_gemma":0.00011570046,"threshold_uncertainty_score":0.006994605},"labels":[],"label_agreement":null},{"id":"W2120114520","doi":"10.1088/0004-637x/815/2/111","title":"MAGNETIC GAMES BETWEEN A PLANET AND ITS HOST STAR: THE KEY ROLE OF TOPOLOGY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planet; Topology (electrical circuits); Angular momentum; Magnetic flux; Magnetic energy; Magnetohydrodynamic drive; Magnetic field; Outer planets; Poynting vector","score_opus":0.013022332909416706,"score_gpt":0.2328167151740587,"score_spread":0.21979438226464199,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120114520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9609743,0.00044304875,0.012045473,0.0005795471,0.000036352987,0.000018398814,0.000051516963,0.000044273806,0.025807034],"genre_scores_gemma":[0.9987367,0.00007797879,0.00060625037,0.000012020178,0.00000867826,0.0000047953517,0.000011474011,0.000006798224,0.0005353693],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993885,0.000023662069,0.0000018672531,0.000009666053,0.000013254977,0.000012728625],"domain_scores_gemma":[0.99977213,0.00006775442,0.000057983165,0.000017410815,0.000015034878,0.000069629525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108144086,0.00017104034,0.00033001488,0.00022794938,0.000658964,0.0014317163,0.00050422974,0.00051075546,0.0018117988],"category_scores_gemma":[0.0012135601,0.00014317315,0.00018891576,0.00018763026,0.0009388309,0.0013556714,0.0009745567,0.00032813443,0.00015886691],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039889975,0.00013273123,0.026706278,0.00013928671,0.00009261698,0.00097047887,0.0006130434,0.80133617,0.015491991,0.14388545,0.0010580203,0.009175009],"study_design_scores_gemma":[0.00010388186,0.00015492736,0.012612539,0.00002528155,0.000030363739,0.0003493667,0.00055027264,0.9428977,0.0014360128,0.037786238,0.004019196,0.00003420623],"about_ca_topic_score_codex":0.0018311631,"about_ca_topic_score_gemma":0.001255848,"teacher_disagreement_score":0.0018311631,"about_ca_system_score_codex":0.00047485385,"about_ca_system_score_gemma":0.0002944525,"threshold_uncertainty_score":0.006061077},"labels":[],"label_agreement":null},{"id":"W2120115896","doi":"10.1086/321475","title":"The Structure and Evolution of Magnetized Cloud Cores in a Zero‐Density Background","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Ambipolar diffusion; Magnetic field; Core (optical fiber); Oblate spheroid; Magnetic cloud; Polar; Gravitational collapse; Magnetohydrodynamics","score_opus":0.008090037770828276,"score_gpt":0.22784564113477615,"score_spread":0.21975560336394787,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120115896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985708,0.000037775164,0.00033456588,0.000036743557,0.000001846593,0.0000031052043,0.000035412042,0.000013606596,0.00096611324],"genre_scores_gemma":[0.99960774,0.00001573282,0.00017552511,0.000007125708,0.00000260438,0.0000013699247,0.00005741944,0.0000043826803,0.00012813836],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999515,0.000004726975,0.00000148351,0.0000118736225,0.000007735448,0.000022749193],"domain_scores_gemma":[0.99982685,0.00001757553,0.000039519913,0.00001076471,0.00002607005,0.0000791518],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012296421,0.00020411593,0.00020707161,0.00035883597,0.000579696,0.0008238731,0.0005683074,0.0002597871,0.00052986445],"category_scores_gemma":[0.00036913666,0.00017030672,0.00015297854,0.00018087264,0.0005468795,0.00036875467,0.0005276969,0.0003096847,0.00008092896],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017022787,0.0005825353,0.33480063,0.00008143981,0.00017352549,0.0034602087,0.0008639721,0.21837968,0.3799452,0.0417391,0.0014140226,0.016857458],"study_design_scores_gemma":[0.00018824513,0.00040842133,0.41775566,0.000021658949,0.00006782317,0.00036081055,0.00043364894,0.5543386,0.019954953,0.0044827126,0.0019212295,0.00006618555],"about_ca_topic_score_codex":0.016107619,"about_ca_topic_score_gemma":0.007241291,"teacher_disagreement_score":0.016107619,"about_ca_system_score_codex":0.0012609294,"about_ca_system_score_gemma":0.00038477228,"threshold_uncertainty_score":0.03202772},"labels":[],"label_agreement":null},{"id":"W2120134498","doi":"10.1088/0004-637x/794/2/171","title":"A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND<i>B</i>-MODE POLARIZATION POWER SPECTRUM AT SUB-DEGREE SCALES WITH POLARBEAR","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":298,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); McGill University; Dalhousie University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; McGill University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Japan Society for the Promotion of Science; Canada Research Chairs; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Cosmic microwave background; Gravitational lens; Multipole expansion; Polarization (electrochemistry); Gravitational wave; Amplitude; Cosmology; Planck; Spectral density","score_opus":0.009363278497752281,"score_gpt":0.2149593146864143,"score_spread":0.205596036188662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120134498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.979882,0.00032802107,0.008679496,0.00012754583,0.000016583419,0.000023731352,0.0029363632,0.00016424742,0.007842064],"genre_scores_gemma":[0.9912635,0.0002434519,0.0057671797,0.000050886196,0.000027399781,0.000030480764,0.0016456662,0.000037675814,0.0009336729],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999811,0.000035024306,0.0000053565514,0.000049860675,0.00007257065,0.000026164134],"domain_scores_gemma":[0.9996294,0.00007356477,0.000108836524,0.00006975961,0.00006190393,0.00005661311],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002815564,0.00025388246,0.0001406514,0.00068167504,0.0001786702,0.00037309644,0.00018973442,0.00015224745,0.0010207512],"category_scores_gemma":[0.00061856426,0.00015582998,0.00011954181,0.00091072405,0.00021096773,0.00031377852,0.0005023671,0.0003130632,0.00040094747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070529577,0.00018435088,0.6767103,0.00022442787,0.00021216978,0.0004060602,0.00045278188,0.0034108155,0.25914583,0.0020351328,0.0023969836,0.05411581],"study_design_scores_gemma":[0.000028790104,0.00018618138,0.9396719,0.000019327194,0.000067073765,0.00039804121,0.0001430911,0.003907514,0.048566747,0.0010295198,0.0059416187,0.00004021485],"about_ca_topic_score_codex":0.0012600241,"about_ca_topic_score_gemma":0.0015638935,"teacher_disagreement_score":0.0012600241,"about_ca_system_score_codex":0.00016713864,"about_ca_system_score_gemma":0.000102721846,"threshold_uncertainty_score":0.0034148097},"labels":[],"label_agreement":null},{"id":"W2120247109","doi":"10.3847/0004-637x/817/1/48","title":"DEEP NEAR-IR OBSERVATIONS OF THE GLOBULAR CLUSTER M4: HUNTING FOR BROWN DWARFS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Globular cluster; Photometry (optics); Brown dwarf; Magnitude (astronomy); White dwarf; Cluster (spacecraft); Near-infrared spectroscopy; Limit (mathematics)","score_opus":0.017690340441431425,"score_gpt":0.22720864746242073,"score_spread":0.2095183070209893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120247109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998879,0.00003505388,0.00015626814,0.000016250313,0.000001758606,0.0000052965197,0.00032225944,0.000018889981,0.0005650739],"genre_scores_gemma":[0.9974082,0.00002620536,0.00090338866,0.000014879991,0.000007698046,0.000006349141,0.0010211295,0.000009695504,0.0006024747],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988174,0.000009742646,0.0000043606815,0.000028214736,0.00003624752,0.00003963154],"domain_scores_gemma":[0.9997029,0.000029138571,0.00006995868,0.00003038929,0.00005850258,0.000109151486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017252039,0.0002696894,0.00024322497,0.0015319977,0.00054725,0.00026606282,0.00034425766,0.00027046935,0.0011404814],"category_scores_gemma":[0.00029265656,0.0001362573,0.00024900853,0.00072417024,0.00025216123,0.00018628562,0.00047841264,0.0001877464,0.00035795686],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006423691,0.00012905046,0.8663098,0.000056275378,0.000100095494,0.0006780083,0.0005766416,0.0012999634,0.11378771,0.00014830391,0.0010826754,0.01518905],"study_design_scores_gemma":[0.0000062511003,0.00007013019,0.9951441,0.0000033768695,0.00001791663,0.00013436332,0.00015296324,0.0008441284,0.002689859,0.00006373028,0.0008668628,0.0000064061983],"about_ca_topic_score_codex":0.010396529,"about_ca_topic_score_gemma":0.01537211,"teacher_disagreement_score":0.010396529,"about_ca_system_score_codex":0.000568986,"about_ca_system_score_gemma":0.00018488221,"threshold_uncertainty_score":0.020672023},"labels":[],"label_agreement":null},{"id":"W2120289895","doi":"10.1086/431925","title":"A Multiwavelength View of the TeV Blazar Markarian 421: Correlated Variability, Flaring, and Spectral Evolution","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":224,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Blazar; Astrophysics; Physics; Astronomy; Gamma ray","score_opus":0.004655289071318336,"score_gpt":0.19872580785339772,"score_spread":0.19407051878207937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120289895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976809,0.00016675946,0.00042279082,0.000039225306,0.000003317455,0.0000037100128,0.00053337996,0.00004969119,0.0011001015],"genre_scores_gemma":[0.9986418,0.000053854077,0.0005452699,0.00001534143,0.000011578055,0.000002989926,0.0005435569,0.000014459836,0.00017114921],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991095,0.000011184173,0.0000052595674,0.000031296688,0.000020546686,0.000020797332],"domain_scores_gemma":[0.99960333,0.00005645329,0.00019153899,0.00004138041,0.000039709324,0.00006770377],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018166927,0.00015907048,0.00017518543,0.0011253918,0.00028815417,0.00040903705,0.00019272686,0.0002262272,0.0006375879],"category_scores_gemma":[0.00029648494,0.00012569418,0.00028671217,0.0008714488,0.00012778013,0.00020131834,0.0003017054,0.00033719867,0.00023212665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037625694,0.000087266504,0.8837539,0.00007861827,0.00020713473,0.0010423874,0.0007215592,0.0014695352,0.09357726,0.000167659,0.0006070589,0.017911317],"study_design_scores_gemma":[0.0000016000538,0.000024655425,0.99772245,0.0000024375279,0.00001720663,0.0002928137,0.00004316087,0.00055504206,0.0009942282,0.000026156682,0.00031597758,0.000004265874],"about_ca_topic_score_codex":0.0022813766,"about_ca_topic_score_gemma":0.004340201,"teacher_disagreement_score":0.0022813766,"about_ca_system_score_codex":0.00018843435,"about_ca_system_score_gemma":0.00006220946,"threshold_uncertainty_score":0.004536152},"labels":[],"label_agreement":null},{"id":"W2120295959","doi":"10.1088/0004-637x/698/2/1934","title":"SPECTROSCOPIC CONFIRMATION OF TWO MASSIVE RED-SEQUENCE-SELECTED GALAXY CLUSTERS AT<i>z</i>∼ 1.2 IN THE SpARCS-NORTH CLUSTER SURVEY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":169,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; University of Waterloo; University of Toronto","funders":"","keywords":"Physics; Cluster (spacecraft); Redshift; Galaxy; Astrophysics; Galaxy cluster; Spectroscopy; Astronomy","score_opus":0.018702771649642753,"score_gpt":0.2549165233830971,"score_spread":0.23621375173345435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120295959","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99874854,0.00005512215,0.00008084779,0.000031478667,0.0000060960074,0.000011395154,0.00014887935,0.000010952917,0.0009066072],"genre_scores_gemma":[0.9987012,0.000038383798,0.00025335845,0.000042404736,0.000009790804,0.000007090876,0.00061442255,0.0000043055284,0.00032904485],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959093,0.000021304242,0.000026565063,0.000118648655,0.00012195562,0.00012064025],"domain_scores_gemma":[0.9987663,0.00007584311,0.00024308875,0.00007201682,0.00020958138,0.00063314114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053858693,0.0003856297,0.0003740571,0.0016179573,0.0010192362,0.00074128615,0.00068097375,0.00037647597,0.0014875656],"category_scores_gemma":[0.00074934034,0.0002917175,0.00025917703,0.0006762133,0.0006618847,0.00022357021,0.0010232754,0.00041263364,0.00053894817],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002645594,0.00008305906,0.9741644,0.000020026262,0.000040345396,0.0009318693,0.0007310093,0.0000937278,0.019761888,0.00027125177,0.0005001856,0.003137601],"study_design_scores_gemma":[0.000015906948,0.00006720908,0.9969597,0.0000045209504,0.000019470725,0.00063938193,0.0002043296,0.000117436706,0.0013385486,0.000031701333,0.0005967774,0.000005149426],"about_ca_topic_score_codex":0.014049022,"about_ca_topic_score_gemma":0.031247541,"teacher_disagreement_score":0.014049022,"about_ca_system_score_codex":0.0007532635,"about_ca_system_score_gemma":0.00043669352,"threshold_uncertainty_score":0.027934492},"labels":[],"label_agreement":null},{"id":"W2120344627","doi":"10.1088/0004-637x/791/2/77","title":"<i>NuSTAR</i>OBSERVATIONS OF THE STATE TRANSITION OF MILLISECOND PULSAR BINARY PSR J1023+0038","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; Canada Research Chairs; California Institute of Technology; Jet Propulsion Laboratory","keywords":"Physics; Millisecond pulsar; Astrophysics; Pulsar; Millisecond; Binary pulsar; Binary number; Astronomy; Pulsar planet","score_opus":0.011750565850226404,"score_gpt":0.2112085450046285,"score_spread":0.19945797915440208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120344627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99594927,0.00021311974,0.00031579167,0.000034947232,0.000012863923,0.000009854518,0.0009400827,0.00013070919,0.0023934222],"genre_scores_gemma":[0.99334794,0.0001608681,0.002054887,0.00006204674,0.00003444008,0.000017473069,0.003497433,0.000032026095,0.0007929434],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986446,0.0000064135274,0.00001058743,0.000037539277,0.000048894373,0.000032070147],"domain_scores_gemma":[0.99967587,0.000014887022,0.00014330771,0.000044731885,0.00004125755,0.0000799097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022583196,0.00025174086,0.00031660742,0.0007546332,0.0003775591,0.00040296375,0.00040049842,0.00033398648,0.00091062725],"category_scores_gemma":[0.0003567434,0.00017317354,0.00023775517,0.0005906578,0.00019196156,0.0003062831,0.0006624493,0.00034074674,0.0004031851],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012962167,0.00028449565,0.5955346,0.00025788072,0.00026160807,0.0022001583,0.0007568791,0.0010950036,0.34472883,0.00040970868,0.003379201,0.049795423],"study_design_scores_gemma":[0.000025327196,0.0003140416,0.9822473,0.000014185904,0.000041351563,0.0017731596,0.000092114955,0.0010921187,0.00952612,0.00011194082,0.0047412743,0.000020944382],"about_ca_topic_score_codex":0.0024123027,"about_ca_topic_score_gemma":0.008749349,"teacher_disagreement_score":0.0024123027,"about_ca_system_score_codex":0.0002800307,"about_ca_system_score_gemma":0.00017882069,"threshold_uncertainty_score":0.0047965646},"labels":[],"label_agreement":null},{"id":"W2120357483","doi":"10.1088/0004-637x/751/1/41","title":"CHARACTERIZING LENSES AND LENSED STARS OF HIGH-MAGNIFICATION SINGLE-LENS GRAVITATIONAL MICROLENSING EVENTS WITH LENSES PASSING OVER SOURCE STARS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Science and Technology Facilities Council; National Research Foundation of Korea; Japan Society for the Promotion of Science; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Fédération Wallonie-Bruxelles; National Research Foundation; National Science Foundation","keywords":"Gravitational microlensing; Physics; Stars; Gravitational lens; Lens (geology); Magnification; Astrophysics; Astronomy; Gravitation; Optics; Galaxy","score_opus":0.015556182782292295,"score_gpt":0.21603784711855786,"score_spread":0.20048166433626557,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120357483","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993192,0.000058661106,0.00012610885,0.0000045911274,9.874909e-7,0.0000046647133,0.00015335748,0.00000605491,0.00032642804],"genre_scores_gemma":[0.9989998,0.000027671169,0.00028156844,0.000005269287,0.000004836034,0.0000022288384,0.00048161973,0.0000033635044,0.00019358171],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997507,0.000016804053,0.000029884932,0.000063231535,0.000077293786,0.00006197607],"domain_scores_gemma":[0.9982608,0.00029491607,0.000693426,0.000088690664,0.00018452066,0.00047763804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000342086,0.00024193739,0.00023600055,0.002322062,0.00040242117,0.0007186767,0.0002479867,0.00029507835,0.0011022893],"category_scores_gemma":[0.0011407563,0.00016286076,0.00033920168,0.001281452,0.00025855162,0.00040916904,0.00081544754,0.00016135337,0.00018406833],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016700223,0.000017676679,0.9882486,0.000010219887,0.000046414927,0.00027327376,0.00015759397,0.000068260226,0.007808859,0.000030854648,0.000034784603,0.0031364101],"study_design_scores_gemma":[0.0000011395724,0.000012235644,0.99905545,6.782618e-7,0.0000078441235,0.00021448855,0.0000729042,0.00009710316,0.00046342672,0.000007876741,0.00006535838,0.0000014831479],"about_ca_topic_score_codex":0.0058381977,"about_ca_topic_score_gemma":0.013168598,"teacher_disagreement_score":0.0058381977,"about_ca_system_score_codex":0.0003916365,"about_ca_system_score_gemma":0.00017059912,"threshold_uncertainty_score":0.011608422},"labels":[],"label_agreement":null},{"id":"W2120515464","doi":"10.1088/0004-637x/770/2/151","title":"ALIGNMENT BETWEEN FLATTENED PROTOSTELLAR INFALL ENVELOPES AND AMBIENT MAGNETIC FIELDS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; Western University","funders":"","keywords":"Magnetic field; Polarization (electrochemistry); Outflow; Rotational symmetry; Symmetry (geometry); Core (optical fiber)","score_opus":0.008554307929006051,"score_gpt":0.21493632411512997,"score_spread":0.20638201618612392,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120515464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918884,0.000028967308,0.00020718898,0.000007416178,6.8143356e-7,0.0000010252539,0.0001105381,0.000023341683,0.0004319845],"genre_scores_gemma":[0.999676,0.000008431656,0.00012128016,0.0000039265287,0.0000015057874,8.27398e-7,0.00014901675,0.000002460904,0.00003655492],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994767,0.0000055090914,0.000002626906,0.000017311591,0.000011415223,0.000015482683],"domain_scores_gemma":[0.9997009,0.000054836783,0.00009829964,0.000027125885,0.000047164278,0.000071687406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008786706,0.00011939473,0.00012540733,0.0006692883,0.00020591688,0.0003702117,0.00014942078,0.00017260794,0.000665284],"category_scores_gemma":[0.0003745679,0.0001069827,0.00008853707,0.00036472685,0.00018351246,0.00017296034,0.0002980147,0.00016605399,0.00014209394],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027941007,0.000034172306,0.9005129,0.00002172271,0.000039960578,0.00031978832,0.00029514765,0.00088800397,0.08902815,0.00019892927,0.0002364065,0.008145442],"study_design_scores_gemma":[0.00000382592,0.000019308802,0.99643433,0.0000017400041,0.000005831478,0.00012361397,0.000064673695,0.0009602694,0.0021927636,0.00006288676,0.00012823968,0.0000026018224],"about_ca_topic_score_codex":0.0012759154,"about_ca_topic_score_gemma":0.0022771356,"teacher_disagreement_score":0.0012759154,"about_ca_system_score_codex":0.00020178012,"about_ca_system_score_gemma":0.00006920124,"threshold_uncertainty_score":0.0025369525},"labels":[],"label_agreement":null},{"id":"W2120579120","doi":"10.1088/0004-637x/799/2/137","title":"MEASUREMENT OF GALAXY CLUSTER INTEGRATED COMPTONIZATION AND MASS SCALING RELATIONS WITH THE SOUTH POLE TELESCOPE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Galaxy cluster; Redshift; RADIUS; Galaxy; Cluster (spacecraft); Sunyaev–Zel'dovich effect; Scaling; South Pole Telescope; Telescope; Aperture (computer memory); Anisotropy; Optics","score_opus":0.01292288099664789,"score_gpt":0.20106120544183662,"score_spread":0.18813832444518871,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120579120","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9846912,0.00035753407,0.0028618686,0.00020859351,0.000021785105,0.000027383052,0.0011080458,0.00013239501,0.010591061],"genre_scores_gemma":[0.99478924,0.00010637665,0.002799953,0.000047664227,0.00001664631,0.000013672017,0.0009251158,0.000025548246,0.001275722],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972004,0.000034735924,0.0000051841416,0.00010775172,0.00009964246,0.000032757373],"domain_scores_gemma":[0.9991874,0.000095939446,0.00015375018,0.00016294996,0.00022612665,0.00017382001],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040537296,0.00017675475,0.0001532609,0.0011806795,0.00046927496,0.0005152134,0.00037910222,0.000243715,0.0012711649],"category_scores_gemma":[0.0011850157,0.00019117138,0.00014615202,0.0011823412,0.0003329777,0.0004366217,0.00064141885,0.00033671357,0.00041050813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000324501,0.000081463586,0.90527153,0.000057643934,0.00012133431,0.00010546646,0.0007829798,0.0010911204,0.048039023,0.0028927424,0.0037648196,0.037467476],"study_design_scores_gemma":[0.000010100037,0.000027451186,0.99318767,0.000004976068,0.000016031081,0.000066752495,0.00009462575,0.0016951878,0.0014608068,0.00037031705,0.0030552733,0.00001085154],"about_ca_topic_score_codex":0.021052161,"about_ca_topic_score_gemma":0.04319976,"teacher_disagreement_score":0.021052161,"about_ca_system_score_codex":0.000816125,"about_ca_system_score_gemma":0.00036463005,"threshold_uncertainty_score":0.04185921},"labels":[],"label_agreement":null},{"id":"W2120645885","doi":"10.3847/0004-637x/817/2/93","title":"NUSTAR OBSERVATIONS OF THE YOUNG, ENERGETIC RADIO PULSAR PSR B1509–58","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Spectral index; Spectral line; Supernova remnant; Photon; Synchrotron; Supernova; Telescope; Light curve","score_opus":0.014810595805546098,"score_gpt":0.216227997789347,"score_spread":0.20141740198380093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120645885","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99621,0.00021868397,0.0012143751,0.0000141686605,0.0000063191037,0.0000061417177,0.00045171974,0.000103379905,0.0017753576],"genre_scores_gemma":[0.99557143,0.000101190715,0.002469339,0.000019904437,0.000010823631,0.000007956298,0.0015049739,0.0000170605,0.00029739592],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999866,0.000015304831,0.000012369268,0.00003595931,0.000056761735,0.000013596494],"domain_scores_gemma":[0.9996562,0.000048255268,0.00012201593,0.00005462451,0.000047692713,0.000071279675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048470974,0.00017307466,0.00024952594,0.0007224955,0.000286392,0.00027214762,0.0002596378,0.00021832928,0.0005533034],"category_scores_gemma":[0.0005501269,0.00017362641,0.000253806,0.0003993393,0.00016125986,0.00021460415,0.00042021854,0.00016338928,0.0003650636],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009925442,0.0001826783,0.71109134,0.0001509719,0.00024842646,0.00063953426,0.00037539098,0.0049541383,0.24407151,0.00074458244,0.0011578333,0.0353911],"study_design_scores_gemma":[0.000034936387,0.00034635514,0.98083067,0.000017887753,0.000043667358,0.00061342906,0.000039143837,0.0053674034,0.010261498,0.00020537071,0.002226398,0.00001331091],"about_ca_topic_score_codex":0.000836911,"about_ca_topic_score_gemma":0.0020869314,"teacher_disagreement_score":0.000836911,"about_ca_system_score_codex":0.00017262618,"about_ca_system_score_gemma":0.00010127237,"threshold_uncertainty_score":0.002563417},"labels":[],"label_agreement":null},{"id":"W2120880319","doi":"10.1088/0004-637x/698/2/1639","title":"BARRED GALAXIES IN THE ABELL 901/2 SUPERCLUSTER WITH STAGES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Waterloo; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration; Austrian Science Fund; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Supercluster (genetic); Astrophysics; Physics; Bulge; Bar (unit); Galaxy; Redshift; Cluster (spacecraft); Galaxy cluster; Astronomy","score_opus":0.006354681619860126,"score_gpt":0.20560920742633912,"score_spread":0.19925452580647898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120880319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996113,0.00002415276,0.000018010278,0.000004604837,4.640725e-7,0.0000016912065,0.00013879164,0.000004433774,0.00019647642],"genre_scores_gemma":[0.9987219,0.00001706094,0.0000890249,0.000009395834,0.0000023505315,0.0000030311082,0.0009361155,0.000004178436,0.00021677131],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972564,0.000019613128,0.000011775831,0.000085716965,0.00006693519,0.00009018683],"domain_scores_gemma":[0.99925894,0.000050971816,0.00030183664,0.000064327636,0.00008110006,0.00024278364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016706598,0.00025888364,0.00027429746,0.0017693755,0.00046487508,0.00070854457,0.00030594307,0.0001996383,0.00076836726],"category_scores_gemma":[0.00050360576,0.00017653713,0.0001991537,0.00095223216,0.0003859924,0.00024801103,0.0007789217,0.00020555886,0.0003223056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014094893,0.000047513247,0.9890127,0.0000064055835,0.000026193704,0.00014910406,0.0002823139,0.00011197301,0.007374839,0.0000696638,0.00018298374,0.002595192],"study_design_scores_gemma":[0.0000019733836,0.000013235555,0.9993692,9.878644e-7,0.0000043859945,0.00007365828,0.000082881896,0.00011619115,0.00020432711,0.0000112461075,0.00012049933,0.0000014807188],"about_ca_topic_score_codex":0.015400559,"about_ca_topic_score_gemma":0.028553879,"teacher_disagreement_score":0.015400559,"about_ca_system_score_codex":0.0005362383,"about_ca_system_score_gemma":0.00018814925,"threshold_uncertainty_score":0.030621827},"labels":[],"label_agreement":null},{"id":"W2120919950","doi":"10.1088/0004-637x/788/2/155","title":"NuSTAR DISCOVERY OF A YOUNG, ENERGETIC PULSAR ASSOCIATED WITH THE LUMINOUS GAMMA-RAY SOURCE HESS J1640–465","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Astrophysics; Gamma ray; Astronomy; Gamma-ray astronomy","score_opus":0.004195473028414218,"score_gpt":0.18341220097960892,"score_spread":0.1792167279511947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2120919950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873906,0.00015452757,0.00018112715,0.000032494136,0.0000073022306,0.0000035045175,0.0001712779,0.000015767644,0.0006949899],"genre_scores_gemma":[0.9982431,0.00010511238,0.0007126759,0.000040375184,0.000013265666,0.000002298981,0.0005328,0.00000345524,0.00034705835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999232,0.0000058323517,0.000007978983,0.000024672627,0.000024523993,0.000013759153],"domain_scores_gemma":[0.99973744,0.000021433172,0.00010392302,0.000029909996,0.000017959172,0.00008929348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001728581,0.00014624653,0.0001326748,0.000499082,0.00035292865,0.0003962449,0.00021867303,0.00041189068,0.00062106515],"category_scores_gemma":[0.00024709385,0.00010478272,0.00012191925,0.0002508632,0.0002294017,0.00023969692,0.00053407275,0.00018855477,0.00028189374],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007799662,0.00008881677,0.67950153,0.000105351486,0.00010027891,0.012951073,0.0007086772,0.0004170759,0.28186586,0.00066316914,0.0006954124,0.022122812],"study_design_scores_gemma":[0.000015930447,0.00037116438,0.95764834,0.000015569243,0.00005049147,0.012897483,0.00028358406,0.00065028376,0.022009142,0.00022636217,0.005811303,0.000020284153],"about_ca_topic_score_codex":0.0007218513,"about_ca_topic_score_gemma":0.0013484232,"teacher_disagreement_score":0.0007218513,"about_ca_system_score_codex":0.00017174258,"about_ca_system_score_gemma":0.0001131762,"threshold_uncertainty_score":0.002077639},"labels":[],"label_agreement":null},{"id":"W2121087773","doi":"10.1088/0004-637x/800/1/61","title":"A SEARCH FOR PULSATIONS FROM GEMINGA ABOVE 100 GeV WITH VERITAS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Pulsar; Fermi Gamma-ray Space Telescope; Context (archaeology); Telescope; Flux (metallurgy); Spectral line; Astronomy","score_opus":0.024395445605295513,"score_gpt":0.2581301234872235,"score_spread":0.23373467788192795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121087773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968624,0.00020247124,0.00057350745,0.00004800838,0.000008990285,0.000010226585,0.0009936991,0.000059104954,0.001241566],"genre_scores_gemma":[0.99393326,0.00007920887,0.0019510263,0.00004502408,0.00002072881,0.00000803434,0.0035336742,0.000017098213,0.0004118002],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996146,0.000039920924,0.000022087253,0.00011214171,0.00011581086,0.00009544456],"domain_scores_gemma":[0.9985929,0.0003336782,0.0005234443,0.00017336539,0.000113037815,0.0002634562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077610137,0.00028867385,0.0002650056,0.0015623829,0.00055069797,0.0006695846,0.00043376524,0.00041995465,0.0015632408],"category_scores_gemma":[0.001215627,0.00027746375,0.0002857731,0.0012924764,0.000276979,0.00032349356,0.00094529835,0.00038328834,0.00025959796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005880231,0.00007573078,0.9348224,0.00005087996,0.0001348692,0.0005677366,0.00031775603,0.0003477822,0.04169052,0.0004086509,0.0007557721,0.020239964],"study_design_scores_gemma":[0.000019334859,0.00019706441,0.9894197,0.000013730331,0.000066451954,0.00071340485,0.000108172026,0.000911167,0.0043677306,0.00014180742,0.004029863,0.00001164667],"about_ca_topic_score_codex":0.0023587605,"about_ca_topic_score_gemma":0.0055104913,"teacher_disagreement_score":0.0023587605,"about_ca_system_score_codex":0.00027951138,"about_ca_system_score_gemma":0.0003451214,"threshold_uncertainty_score":0.0052295923},"labels":[],"label_agreement":null},{"id":"W2121129108","doi":"10.1088/0004-637x/723/2/1583","title":"A PRECISE ASTEROSEISMIC AGE AND RADIUS FOR THE EVOLVED SUN-LIKE STAR KIC 11026764","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency","funders":"Science and Technology Facilities Council","keywords":"Subgiant; Exoplanet; Photometry (optics); Physics; Asteroseismology; Kepler; Stars; Planet; RADIUS; Oscillation (cell signaling); Astrophysics; Astronomy; Circumstellar habitable zone; Globular cluster; Computer science","score_opus":0.01153274291323806,"score_gpt":0.22622166547543596,"score_spread":0.2146889225621979,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121129108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925011,0.00028800094,0.0038437427,0.00004914154,0.000008680501,0.000015488118,0.00093657867,0.00009364692,0.0022636983],"genre_scores_gemma":[0.99392104,0.000104163206,0.004103953,0.000008514685,0.0000034656755,0.000009234876,0.0014372582,0.00003536621,0.00037709405],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985385,0.000014625956,0.000009335419,0.000059757363,0.0000438974,0.000018593268],"domain_scores_gemma":[0.9996563,0.00004931555,0.000107352425,0.00006462641,0.00007909704,0.00004324981],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003731535,0.00037557213,0.00032449185,0.0009955439,0.0007574712,0.00063091534,0.00063209777,0.0003921672,0.0006960943],"category_scores_gemma":[0.0009604567,0.00032769394,0.00039272124,0.00092208403,0.00035401693,0.00055142934,0.00044514608,0.00029203168,0.00046264284],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041065132,0.000090301,0.7068347,0.00016333349,0.0001624237,0.00047971372,0.00037888013,0.19896002,0.06683776,0.0037654564,0.0013739297,0.020542849],"study_design_scores_gemma":[0.000090506815,0.00014753621,0.6757059,0.00004514859,0.0001167241,0.00043467266,0.00027365668,0.2805837,0.032212988,0.002078471,0.008176408,0.00013426984],"about_ca_topic_score_codex":0.024714159,"about_ca_topic_score_gemma":0.024908379,"teacher_disagreement_score":0.024714159,"about_ca_system_score_codex":0.0018614838,"about_ca_system_score_gemma":0.0008038388,"threshold_uncertainty_score":0.049140632},"labels":[],"label_agreement":null},{"id":"W2121156627","doi":"10.1086/344082","title":"PSR J2021+3651: A Young Radio Pulsar Coincident with an Unidentified EGRET γ-Ray Source","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Luminosity; Egret; Astronomy; Nebula; Source counts; Pulsar wind nebula; Galaxy; Gamma ray","score_opus":0.00991834581490417,"score_gpt":0.20529683682492814,"score_spread":0.19537849101002397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121156627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977069,0.00024887294,0.000452969,0.000056112225,0.000017997476,0.00001753427,0.00022494605,0.00003239731,0.0012422915],"genre_scores_gemma":[0.99716467,0.00019228824,0.0008918127,0.00008291599,0.000031743708,0.000006924961,0.0008171981,0.000006993432,0.0008054783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978906,0.00001198552,0.000019294117,0.00006376937,0.00006396531,0.000051924242],"domain_scores_gemma":[0.99956864,0.0000367915,0.00015614921,0.00003925626,0.000028180359,0.00017109058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018519696,0.0005763299,0.00037765718,0.0012814746,0.0011069076,0.0009661452,0.00045911747,0.0005579027,0.0013302483],"category_scores_gemma":[0.00032146688,0.00020901558,0.0003445494,0.0009648054,0.00043660132,0.00034996553,0.0008815579,0.00044687817,0.00075864396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006586764,0.00024634786,0.852846,0.00020216443,0.00009777702,0.025799563,0.001787427,0.0006233359,0.077320196,0.0005870105,0.00088068005,0.038950913],"study_design_scores_gemma":[0.000038643226,0.0012667425,0.9546732,0.00004268076,0.00014354236,0.017132014,0.0011458239,0.000647956,0.013792807,0.0003039128,0.010764841,0.00004789427],"about_ca_topic_score_codex":0.002232437,"about_ca_topic_score_gemma":0.003913353,"teacher_disagreement_score":0.002232437,"about_ca_system_score_codex":0.00025451067,"about_ca_system_score_gemma":0.00024584672,"threshold_uncertainty_score":0.0044501424},"labels":[],"label_agreement":null},{"id":"W2121268712","doi":"10.1086/341257","title":"Bayesian Analysis of Radio Observations of the Be X‐Ray Binary LS I +61o303","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Modulation (music); Spectral index; Amplitude; Orbital period; Binary number; Be star; Phase (matter); X-ray binary; Synchrotron; Spectral line; Astronomy; Stars; Neutron star; Optics","score_opus":0.02609195419711549,"score_gpt":0.2298945353812693,"score_spread":0.2038025811841538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121268712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906136,0.00011368036,0.008545928,0.00008126399,0.0000028481368,0.000006474554,0.0001224993,0.000045754612,0.0004679728],"genre_scores_gemma":[0.99683917,0.00007251384,0.0023739578,0.000014930947,0.000012576486,0.00000776491,0.00050593854,0.000011084008,0.00016211277],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992368,0.0003095433,0.000051229414,0.0001346175,0.00017082594,0.00009694414],"domain_scores_gemma":[0.99502385,0.0025798725,0.0013646035,0.00036754084,0.0004398978,0.00022424765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002227494,0.00022516951,0.0004560367,0.0010304379,0.00034829302,0.00081552216,0.00044960613,0.0004260925,0.00042125268],"category_scores_gemma":[0.012035701,0.000515428,0.00031464128,0.00058964954,0.00040763296,0.0004893855,0.00067012536,0.000549085,0.00015961137],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022069656,0.00032775782,0.63430214,0.0001736835,0.000572963,0.0006087746,0.0007092166,0.19595167,0.04443233,0.008858348,0.0014073579,0.11044888],"study_design_scores_gemma":[0.000075553835,0.00010442848,0.5029958,0.000018671552,0.000088748166,0.00016252437,0.000104346545,0.48792112,0.0029375062,0.0048357313,0.0006933133,0.00006215671],"about_ca_topic_score_codex":0.007832146,"about_ca_topic_score_gemma":0.008698641,"teacher_disagreement_score":0.007832146,"about_ca_system_score_codex":0.0005648004,"about_ca_system_score_gemma":0.00048917887,"threshold_uncertainty_score":0.015573084},"labels":[],"label_agreement":null},{"id":"W2121325661","doi":"10.1088/0004-637x/779/2/152","title":"CONSTRAINT ON THE POLARIZATION OF ELECTRIC DIPOLE EMISSION FROM SPINNING DUST","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Polarization (electrochemistry); Astrophysics; Stars; Silicate; Planck; Dipole; Cosmic dust; Radiation; Linear polarization; Anisotropy; Astronomy; Optics; Chemistry","score_opus":0.009376327834347642,"score_gpt":0.21993866155915837,"score_spread":0.21056233372481073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121325661","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99131775,0.00006757337,0.006701587,0.000044937216,0.000004350348,0.00000434883,0.0002295266,0.000045455432,0.0015844178],"genre_scores_gemma":[0.99882764,0.000048846465,0.0007555352,0.000010111058,0.000005932421,0.000003893706,0.00027015086,0.000007055897,0.00007078851],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976414,0.000045634795,0.000010847031,0.00006757616,0.000047926762,0.000063919986],"domain_scores_gemma":[0.9992003,0.00036739363,0.00015580063,0.00012459843,0.00007130753,0.00008063613],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003436589,0.0004928657,0.00034873205,0.00044266006,0.0003966287,0.000700599,0.00047174058,0.00046461695,0.0008799616],"category_scores_gemma":[0.0012180174,0.00035036576,0.0005034241,0.0003749459,0.00046857103,0.00040430087,0.00039865653,0.00031540534,0.00020368665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059090037,0.0001567493,0.53920525,0.00010688131,0.00018778784,0.00085831387,0.00018593381,0.29836783,0.13097289,0.014340998,0.00091591955,0.014110583],"study_design_scores_gemma":[0.00011156452,0.00015773637,0.2298251,0.000024894953,0.00010993274,0.00032148018,0.00018239496,0.7221644,0.035522602,0.009753686,0.0017566291,0.000069593196],"about_ca_topic_score_codex":0.00561034,"about_ca_topic_score_gemma":0.0036439141,"teacher_disagreement_score":0.00561034,"about_ca_system_score_codex":0.0005534123,"about_ca_system_score_gemma":0.000498471,"threshold_uncertainty_score":0.011155367},"labels":[],"label_agreement":null},{"id":"W2121398351","doi":"10.1086/320913","title":"On the Origin of Infrared Plateau Features in Proto–Planetary Nebulae","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":131,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Canada Council for the Arts; University of Calgary","funders":"","keywords":"Planetary nebula; Plateau (mathematics); Physics; Infrared; Astrophysics; Observatory; Astronomy; Astrobiology; Astrochemistry; Stars; Interstellar medium; Galaxy","score_opus":0.011307538620352,"score_gpt":0.23960646370978958,"score_spread":0.22829892508943758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121398351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99023527,0.0010009693,0.00095543725,0.000092436414,0.000005147371,0.000011529099,0.00006926932,0.000051604187,0.007578232],"genre_scores_gemma":[0.9985073,0.00029700834,0.00057196023,0.00003337484,0.000011760527,0.0000070966153,0.000111990885,0.000011825689,0.00044758734],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999951,0.0000054475345,0.0000018556551,0.00001517538,0.000009551242,0.000016893877],"domain_scores_gemma":[0.9996505,0.00010880509,0.000085969536,0.00004066843,0.000059441947,0.000054656608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021896469,0.00015729551,0.00014761505,0.00068631564,0.00048887474,0.0006508965,0.00040384344,0.00044225514,0.0017641481],"category_scores_gemma":[0.000667153,0.00019275022,0.00017008782,0.00035504525,0.0006395016,0.0005919724,0.00047464293,0.00043724768,0.0005947069],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014780391,0.00027175425,0.37170202,0.00030057054,0.000060356087,0.004422696,0.0027004073,0.0025429712,0.5133535,0.014123045,0.0013183983,0.08772623],"study_design_scores_gemma":[0.000035555622,0.00022353197,0.968728,0.00005525259,0.000024383362,0.0018488406,0.00040563455,0.002201569,0.016401267,0.0049156547,0.005140657,0.00001968807],"about_ca_topic_score_codex":0.0010069396,"about_ca_topic_score_gemma":0.00075136044,"teacher_disagreement_score":0.0017641481,"about_ca_system_score_codex":0.00029887198,"about_ca_system_score_gemma":0.00011904254,"threshold_uncertainty_score":0.0059016943},"labels":[],"label_agreement":null},{"id":"W2121427473","doi":"10.1088/0004-637x/742/1/9","title":"THEORETICAL<i>p</i>-MODE OSCILLATION FREQUENCIES FOR THE RAPIDLY ROTATING δ SCUTI STAR α OPHIUCHI","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Legendre polynomials; Rotational symmetry; Oscillation (cell signaling); Legendre function; Rotation (mathematics); Space (punctuation); Mode (computer interface); Star (game theory); Stellar rotation","score_opus":0.02038887286614689,"score_gpt":0.2401127168700189,"score_spread":0.21972384400387202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121427473","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98360056,0.00006861917,0.0086456025,0.00008976732,0.000010646677,0.000014968699,0.000502388,0.00015648654,0.00691093],"genre_scores_gemma":[0.99593395,0.000041498923,0.0031339016,0.0000070738647,0.0000024049007,0.000013878396,0.00043346337,0.00003571516,0.00039822917],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995124,0.00000672951,0.0000022465,0.000014643629,0.000014108935,0.000011072866],"domain_scores_gemma":[0.9998934,0.000027722032,0.000022745075,0.000016073118,0.000022855838,0.000017059821],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016870696,0.00035332268,0.00012576743,0.00058707385,0.0004712321,0.00036815245,0.0004481069,0.00047663422,0.0013461424],"category_scores_gemma":[0.0006578085,0.00018596955,0.00039527664,0.000490939,0.0002734066,0.00028674852,0.00018480237,0.00029077925,0.0002740021],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025295955,0.000116252515,0.13889718,0.0001789202,0.00005047778,0.0005820772,0.0004839104,0.75058496,0.05260956,0.024389207,0.0024756042,0.029378906],"study_design_scores_gemma":[0.000042783173,0.00008437254,0.06994488,0.00002081618,0.000015751408,0.00025531786,0.00016483336,0.9179646,0.0043080724,0.00577585,0.0013931172,0.000029781539],"about_ca_topic_score_codex":0.007333066,"about_ca_topic_score_gemma":0.0041303243,"teacher_disagreement_score":0.007333066,"about_ca_system_score_codex":0.0008536003,"about_ca_system_score_gemma":0.0003211394,"threshold_uncertainty_score":0.014580786},"labels":[],"label_agreement":null},{"id":"W2121460726","doi":"10.1088/0004-637x/739/2/94","title":"THE 2009 OUTBURST OF MAGNETAR 1E 1547--5408: PERSISTENT RADIATIVE AND BURST PROPERTIES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Astrophysics; Physics; Flux (metallurgy); Context (archaeology); Radiative transfer; Telescope; Pulsar; Materials science; Geology; Optics","score_opus":0.025663397629368458,"score_gpt":0.26124564305556064,"score_spread":0.2355822454261922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121460726","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995684,0.000035628535,0.0000651103,0.000008667126,0.0000014297235,0.0000014317264,0.00010427661,0.0000059801264,0.00020897022],"genre_scores_gemma":[0.99917287,0.000036687397,0.00010087817,0.000007672236,0.000006983406,0.0000026916214,0.0005236998,0.0000057213106,0.00014274594],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999167,0.000008307702,0.000008722403,0.00002710412,0.000016175905,0.000022977994],"domain_scores_gemma":[0.99928135,0.00012130978,0.0003342211,0.00007158123,0.00008541095,0.00010610262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019691934,0.0001504437,0.00028910738,0.0006105076,0.0003115967,0.00039920662,0.00021932095,0.00015766415,0.00048003838],"category_scores_gemma":[0.00062732084,0.0001095394,0.0001580504,0.00041439492,0.00023269127,0.0002211942,0.00043314666,0.00023532848,0.00014625602],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003277901,0.00005061845,0.9460996,0.000031568285,0.00005555237,0.00042534317,0.0002687853,0.00036397038,0.043320507,0.00013570601,0.00022037385,0.008700189],"study_design_scores_gemma":[0.0000020296854,0.000038539536,0.9985135,0.0000013461757,0.000008299985,0.00020473983,0.000043075386,0.00023349043,0.00076612027,0.000020107862,0.00016600476,0.0000027131096],"about_ca_topic_score_codex":0.0017653089,"about_ca_topic_score_gemma":0.004306931,"teacher_disagreement_score":0.0017653089,"about_ca_system_score_codex":0.00024599937,"about_ca_system_score_gemma":0.000071873765,"threshold_uncertainty_score":0.003510058},"labels":[],"label_agreement":null},{"id":"W2121490738","doi":"10.1088/0004-637x/753/2/158","title":"<i>HST</i>AND OPTICAL DATA REVEAL WHITE DWARF COOLING, SPIN, AND PERIODICITIES IN GW LIBRAE 3-4 YEARS AFTER OUTBURST","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Heritage","funders":"Marsden Fund; M.J. Murdock Charitable Trust; National Aeronautics and Space Administration; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"White dwarf; Physics; Astrophysics; Amplitude; Multiplet; Dwarf nova; Redshift; RADIUS; Spectral line; Astronomy; Hubble space telescope; Effective temperature; Intermediate polar; Stars; Optics; Galaxy","score_opus":0.018281165703733785,"score_gpt":0.24672934075580935,"score_spread":0.22844817505207557,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121490738","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99811065,0.000059329337,0.000047384092,0.000017973709,0.0000027466117,0.0000017011508,0.0007624375,0.00001271493,0.0009851143],"genre_scores_gemma":[0.99662966,0.00006237253,0.00010453824,0.000033479573,0.00001070933,0.0000038004443,0.0025258528,0.0000053560316,0.00062426715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999604,0.0000025680895,0.000003860534,0.000010054763,0.00001011525,0.000013052161],"domain_scores_gemma":[0.9996679,0.000024708728,0.00016469431,0.000022295138,0.000041510397,0.00007896123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009093853,0.00009928765,0.00013132975,0.0006048137,0.000172044,0.00041329916,0.00010160871,0.00016049224,0.0015119215],"category_scores_gemma":[0.0002533184,0.00005950725,0.00010823539,0.0005347385,0.00016854488,0.00016923284,0.00017418472,0.0002129582,0.00034334417],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029881578,0.000069291906,0.9629299,0.000018986508,0.000030476707,0.00047898767,0.00021571493,0.0001223178,0.02715804,0.000096451964,0.00076582754,0.007815249],"study_design_scores_gemma":[4.840976e-7,0.000010165214,0.9994605,7.6228275e-7,0.0000013506868,0.00007509629,0.000025582485,0.000020013067,0.00027043445,0.000007970106,0.00012696072,6.071817e-7],"about_ca_topic_score_codex":0.0039177756,"about_ca_topic_score_gemma":0.009916758,"teacher_disagreement_score":0.0039177756,"about_ca_system_score_codex":0.0001446436,"about_ca_system_score_gemma":0.000069870766,"threshold_uncertainty_score":0.0077899694},"labels":[],"label_agreement":null},{"id":"W2121494879","doi":"10.1086/508369","title":"Long-Wavelength Excesses in Two Highly Obscured High-Mass X-Ray Binaries: IGR J16318-4848 and GX 301-2","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Infrared; Astronomy; Spectral line; X-ray; Wavelength; Neutron star; Optics","score_opus":0.008386908928735115,"score_gpt":0.2270715165247844,"score_spread":0.2186846075960493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121494879","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963844,0.000059732523,0.00004881675,0.000008474791,0.0000012678315,8.617346e-7,0.000048602833,0.000010484049,0.00018321311],"genre_scores_gemma":[0.9995672,0.000023285897,0.00012923546,0.000010219998,0.0000052183855,0.0000017450587,0.00019101347,0.0000045469324,0.00006749632],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991,0.000008804499,0.000007231768,0.000028549952,0.000019825582,0.000025548923],"domain_scores_gemma":[0.99958473,0.000038956932,0.00020113614,0.000038634418,0.000021377215,0.00011519409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018652769,0.00030292518,0.0003439119,0.00067744794,0.0003124591,0.0004806405,0.0003710602,0.0004050879,0.0011973993],"category_scores_gemma":[0.00028747474,0.00015270368,0.0001866419,0.0004974249,0.00025813535,0.00026470155,0.0005600143,0.00027601578,0.00032437863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008073637,0.0001301043,0.9066907,0.000051590083,0.000110680376,0.0009826617,0.00030438337,0.00032278307,0.08392277,0.00021231438,0.00028988929,0.006174798],"study_design_scores_gemma":[0.000015233961,0.000056537105,0.9966654,0.000002942886,0.000021346314,0.0005003935,0.00006683245,0.0005074741,0.0018110438,0.00010515164,0.00024292537,0.0000045724028],"about_ca_topic_score_codex":0.0008943008,"about_ca_topic_score_gemma":0.0018520957,"teacher_disagreement_score":0.0011973993,"about_ca_system_score_codex":0.00026255706,"about_ca_system_score_gemma":0.00004414156,"threshold_uncertainty_score":0.0040056705},"labels":[],"label_agreement":null},{"id":"W2121612392","doi":"10.1086/521997","title":"Bubble Wrap for Bullets: The Stability Imparted by a Thin Magnetic Layer","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Magnetic confinement fusion research","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cluster (spacecraft); Shear (geology); Layer (electronics); Magnetic field; Core (optical fiber); Bubble; Thin layer; Mechanics; Instability; Physics; Wavelength; Granular layer; Work (physics); Condensed matter physics; Materials science; Optics; Nanotechnology; Composite material; Thermodynamics; Computer science","score_opus":0.01691808529699741,"score_gpt":0.2764406257010346,"score_spread":0.2595225404040372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121612392","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9718391,0.00083564414,0.01780411,0.00048359917,0.00012406985,0.00003276978,0.00010507282,0.00045357188,0.008322122],"genre_scores_gemma":[0.9945686,0.00012011003,0.0029136525,0.000077591474,0.000018988387,0.000012516885,0.000062455285,0.00007860424,0.0021475118],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999025,0.000009029001,0.0000030657818,0.000017397717,0.000022688779,0.000045384157],"domain_scores_gemma":[0.99950445,0.00014651254,0.00009029441,0.000037929272,0.00007121721,0.00014948391],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022144913,0.00034448795,0.0004814356,0.00044865336,0.0009043304,0.0013141299,0.00045074246,0.0007782269,0.0037112178],"category_scores_gemma":[0.0016980981,0.00035885308,0.00039824191,0.0001227709,0.00084356184,0.0010119024,0.0011021711,0.0005510647,0.00041002355],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014921263,0.00027282943,0.016650945,0.00044128307,0.00022758893,0.002273734,0.0010825846,0.30833447,0.5879681,0.051572334,0.004991528,0.02469252],"study_design_scores_gemma":[0.00017113223,0.0003093318,0.009499321,0.000034646077,0.00006551368,0.00028780315,0.00022729051,0.93446714,0.0435935,0.008380219,0.0028926872,0.00007138003],"about_ca_topic_score_codex":0.006556673,"about_ca_topic_score_gemma":0.0026203403,"teacher_disagreement_score":0.006556673,"about_ca_system_score_codex":0.0007337557,"about_ca_system_score_gemma":0.00046147694,"threshold_uncertainty_score":0.013036966},"labels":[],"label_agreement":null},{"id":"W2121614080","doi":"10.1088/0004-637x/728/1/35","title":"INCREASING THE FISHER INFORMATION CONTENT IN THE MATTER POWER SPECTRUM BY NONLINEAR WAVELET WIENER FILTERING","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Wavelet; Spectral density; Gaussian; Filter (signal processing); Spectrum (functional analysis); Content (measure theory); Nonlinear system; Set (abstract data type)","score_opus":0.012182832044726677,"score_gpt":0.20845261226534934,"score_spread":0.19626978022062266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121614080","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.15453984,0.000084502506,0.84275734,0.00020187485,0.00001648504,0.000016040001,0.00003192601,0.00016450357,0.0021873743],"genre_scores_gemma":[0.78631496,0.00026571605,0.21053587,0.000075265896,0.000030279163,0.000037173177,0.00006516789,0.00008790004,0.002587601],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989283,0.000030487443,0.000005916193,0.000015600952,0.000037972855,0.000017139751],"domain_scores_gemma":[0.9993724,0.00040132992,0.00008188983,0.00007876666,0.000044159366,0.000021430638],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007795804,0.00040316934,0.0002953933,0.00033422568,0.00018543692,0.00046074376,0.00035539336,0.00045535498,0.0011789337],"category_scores_gemma":[0.0026498465,0.0002439477,0.00041602843,0.00027027423,0.0008482073,0.0011893117,0.0007016199,0.00054809224,0.0002339107],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000208851,0.00009219953,0.0014926542,0.00013385432,0.000058867063,0.0001643962,0.00016759674,0.71040237,0.089008614,0.13304418,0.0004917078,0.06473468],"study_design_scores_gemma":[0.0000073204737,0.000025977006,0.0002495485,0.000003960875,0.0000055567457,0.000014648776,0.0000052074947,0.9813799,0.0063971393,0.011724236,0.00017747474,0.000009055006],"about_ca_topic_score_codex":0.001145527,"about_ca_topic_score_gemma":0.0011659114,"teacher_disagreement_score":0.0011789337,"about_ca_system_score_codex":0.0003575887,"about_ca_system_score_gemma":0.00034339263,"threshold_uncertainty_score":0.004122913},"labels":[],"label_agreement":null},{"id":"W2121647916","doi":"10.1088/0004-637x/755/2/91","title":"CHARACTERIZING LOW-MASS BINARIES FROM OBSERVATION OF LONG-TIMESCALE CAUSTIC-CROSSING GRAVITATIONAL MICROLENSING EVENTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Physics; Einstein radius; Light curve; Caustic (mathematics); Astrophysics; Astronomy; Binary number; RADIUS; Binary star; Gravitational lens; Stars; Galaxy","score_opus":0.01685382019020872,"score_gpt":0.23823903194554238,"score_spread":0.22138521175533366,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121647916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873036,0.00013797639,0.00048996997,0.0000060783764,0.0000019825802,0.0000083077275,0.00014696547,0.000017723913,0.00046048264],"genre_scores_gemma":[0.99890876,0.00003953826,0.00048847194,0.0000076480255,0.0000042887746,0.0000034789969,0.0004397265,0.0000048346205,0.00010326558],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982846,0.000011351141,0.000015324618,0.000047292,0.00004622248,0.000051282084],"domain_scores_gemma":[0.99920815,0.000075542666,0.00038229837,0.00004798305,0.000068558795,0.00021750966],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026086555,0.00020702464,0.0003042325,0.0020763148,0.0003440049,0.0007505493,0.00025268566,0.0002979954,0.0007574813],"category_scores_gemma":[0.0006923342,0.00013604283,0.00016909816,0.0009723646,0.00020318814,0.00038079842,0.00080834806,0.00021130714,0.00027290266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002455941,0.00004848142,0.94174725,0.000029692908,0.0000376874,0.00038714998,0.0002772284,0.0001911456,0.048232477,0.00019734641,0.000094715484,0.00851127],"study_design_scores_gemma":[0.0000023631067,0.00002392583,0.9963082,0.0000028645259,0.000010405239,0.00032397202,0.000074370655,0.00062312407,0.0023725503,0.00006628309,0.00018770728,0.0000042547686],"about_ca_topic_score_codex":0.0022178635,"about_ca_topic_score_gemma":0.0044953893,"teacher_disagreement_score":0.0022178635,"about_ca_system_score_codex":0.00037309766,"about_ca_system_score_gemma":0.00013151423,"threshold_uncertainty_score":0.004409969},"labels":[],"label_agreement":null},{"id":"W2121885109","doi":"10.1086/504634","title":"Discovery of the New Slowly Pulsating B Star HD 163830 (B5 II/III) from <i>MOST</i> Space-based Photometry","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Université de Montréal; Saint Mary's University; St. Mary's University; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; KU Leuven; Austrian Science Fund","keywords":"Physics; Photometry (optics); Stars; Amplitude; Astrophysics; Star (game theory); Astronomy; Optics","score_opus":0.006736598908000006,"score_gpt":0.20266233028758912,"score_spread":0.1959257313795891,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2121885109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99531186,0.0006357817,0.0012453137,0.0000971991,0.000025678362,0.00001613617,0.000335244,0.000060818573,0.0022720778],"genre_scores_gemma":[0.9953778,0.00018255839,0.0029177046,0.00017621553,0.000034035842,0.000010528447,0.00077147497,0.0000146441325,0.0005149227],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998895,0.000010134423,0.000010134751,0.000034607358,0.000035985442,0.000019619823],"domain_scores_gemma":[0.99953914,0.000040848994,0.00015562607,0.00004076124,0.000046227487,0.00017741523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035271994,0.00023067337,0.0002934811,0.00063181284,0.00045173868,0.00065536366,0.00026431092,0.00049879326,0.00077610026],"category_scores_gemma":[0.00047395256,0.00019743279,0.000202962,0.00041578818,0.0003311337,0.00030339512,0.00050164456,0.00044738434,0.00058178295],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006237652,0.00015295006,0.36025152,0.00024516732,0.00011436982,0.002450349,0.000770677,0.00036986868,0.5865578,0.0012872289,0.0019509858,0.045225266],"study_design_scores_gemma":[0.00005112761,0.00070912985,0.9509632,0.000036930498,0.000094316136,0.005519647,0.0002083838,0.00098967,0.02815155,0.00060940825,0.0126399305,0.000026671116],"about_ca_topic_score_codex":0.0007070788,"about_ca_topic_score_gemma":0.0011584663,"teacher_disagreement_score":0.00077610026,"about_ca_system_score_codex":0.00024267183,"about_ca_system_score_gemma":0.00018457255,"threshold_uncertainty_score":0.0025963783},"labels":[],"label_agreement":null},{"id":"W2122011806","doi":"10.1088/0004-637x/749/2/112","title":"A TRANSIENT SUB-EDDINGTON BLACK HOLE X-RAY BINARY CANDIDATE IN THE DUST LANES OF CENTAURUS A","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Alberta","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Neutron star; X-ray transient; Black hole (networking); Black-body radiation; X-ray binary; Galaxy; Astronomy; Luminosity; Compact star; Intermediate-mass black hole; X-ray burster; Stellar black hole; Eddington luminosity; Flux (metallurgy); Binary black hole; Radiation; Stellar evolution; Gravitational wave; Stars; Stellar mass loss","score_opus":0.013492657950957474,"score_gpt":0.2353652514310457,"score_spread":0.22187259348008823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122011806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99693584,0.00016411612,0.00024047936,0.00015869619,0.000051116414,0.0000119813985,0.00006663653,0.000028479342,0.0023426472],"genre_scores_gemma":[0.9991628,0.00002514345,0.00009114091,0.000038625072,0.00003789797,0.0000021216858,0.000044427215,0.0000065000595,0.0005913974],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998611,0.000008322537,0.000011739176,0.00003691246,0.000017438308,0.00006457662],"domain_scores_gemma":[0.9995127,0.000073650386,0.00008783613,0.000044153392,0.000029767776,0.0002519082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018982707,0.000516641,0.0005409479,0.0018017447,0.0014402157,0.0018912185,0.00082425115,0.0013818331,0.006779116],"category_scores_gemma":[0.0009720728,0.00035057156,0.00034816103,0.0005228768,0.0007062232,0.0006546954,0.0011993644,0.0005294051,0.0018059965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002400787,0.00078894116,0.58857965,0.00011469282,0.00008223834,0.31154415,0.0019113229,0.00030093009,0.07174427,0.0030276682,0.0023751254,0.017130215],"study_design_scores_gemma":[0.00011957833,0.0014111523,0.7477758,0.000055962348,0.00011139625,0.2305626,0.0022034708,0.0016081298,0.010496644,0.0023231525,0.0032781377,0.00005399078],"about_ca_topic_score_codex":0.0006645566,"about_ca_topic_score_gemma":0.00086010824,"teacher_disagreement_score":0.006779116,"about_ca_system_score_codex":0.00024814892,"about_ca_system_score_gemma":0.00011200626,"threshold_uncertainty_score":0.022678375},"labels":[],"label_agreement":null},{"id":"W2122139425","doi":"10.1086/592555","title":"The Ghost of a Dwarf Galaxy: Fossils of the Hierarchical Formation of the Nearby Spiral Galaxy NGC 5907","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":160,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Galaxy; Dwarf galaxy; Astronomy; Interacting galaxy; Galactic halo; Accretion (finance); Dwarf spheroidal galaxy; Spiral galaxy; Halo","score_opus":0.00960094557988925,"score_gpt":0.21094116939607968,"score_spread":0.20134022381619043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122139425","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9909889,0.00013548453,0.0021030863,0.00025881172,0.000012241985,0.000006399222,0.00020538953,0.000075644166,0.0062140236],"genre_scores_gemma":[0.9976162,0.00007668423,0.0013251129,0.000044339922,0.0000047059348,0.0000038420076,0.00014219823,0.000018911169,0.00076803635],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99996567,0.000009546137,0.0000013734114,0.0000067386813,0.000008486058,0.000008106231],"domain_scores_gemma":[0.9998846,0.000025213185,0.000021183212,0.000020860089,0.000010767119,0.000037416936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009619144,0.00017108668,0.00025291656,0.00023475054,0.0004653288,0.0007016149,0.00042824398,0.0004902266,0.0016728473],"category_scores_gemma":[0.00045665816,0.00011840415,0.00024676023,0.00022741471,0.0006207592,0.00045421722,0.00064971094,0.0003728221,0.00018054148],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000601526,0.00027776518,0.2455183,0.00022943488,0.00021838497,0.0028576464,0.002251229,0.61635816,0.034315873,0.07033367,0.0057278015,0.021310274],"study_design_scores_gemma":[0.00009162659,0.00034245136,0.15551634,0.000066706445,0.0000901978,0.00073544215,0.0009917998,0.8105059,0.0021009932,0.020788694,0.008708172,0.000061578925],"about_ca_topic_score_codex":0.015622259,"about_ca_topic_score_gemma":0.01721669,"teacher_disagreement_score":0.015622259,"about_ca_system_score_codex":0.000670693,"about_ca_system_score_gemma":0.00041879408,"threshold_uncertainty_score":0.031062663},"labels":[],"label_agreement":null},{"id":"W2122236540","doi":"10.1086/587122","title":"Average Properties of a Large Sample of<i>z</i><sub>abs</sub>∼<i>z</i><sub>em</sub>Associated Mg<scp>ii</scp>Absorption Line Systems","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"QSOS; Astrophysics; Physics; Spectral line; Ionization; Extinction (optical mineralogy); Absorption (acoustics); Absorption spectroscopy; Quasar; Line (geometry); Galaxy; Astronomy; Optics","score_opus":0.010989389164559243,"score_gpt":0.19090665874691823,"score_spread":0.17991726958235899,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122236540","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989073,0.000059816997,0.00041584708,0.000005163163,7.224416e-7,0.000003403266,0.00028089227,0.000014679769,0.00031207709],"genre_scores_gemma":[0.9977137,0.00005394069,0.0004553914,0.000008744702,0.0000059197155,0.0000048730026,0.0015454422,0.000013825029,0.00019819112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977857,0.000018269862,0.000016236387,0.00009831468,0.000049393835,0.00003931775],"domain_scores_gemma":[0.99915934,0.00022017956,0.00018392815,0.00013257515,0.0001854775,0.00011850901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033122682,0.0001545578,0.00024391912,0.00086218375,0.00032989506,0.0005167141,0.00023664247,0.0002072235,0.0011559966],"category_scores_gemma":[0.0010560971,0.0001270869,0.00022615063,0.00088733435,0.00022355147,0.00049222226,0.00033530762,0.00015348686,0.00034236116],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024994722,0.00009784808,0.8813702,0.00005849276,0.00019271353,0.0002487582,0.0004599628,0.0019005149,0.09997035,0.00020129653,0.00033939438,0.014910556],"study_design_scores_gemma":[0.0000036144645,0.00009643119,0.9910495,0.0000016022916,0.000043128755,0.0002831358,0.00012984443,0.001722754,0.0058619846,0.0000715255,0.0007304899,0.0000059803497],"about_ca_topic_score_codex":0.0016288131,"about_ca_topic_score_gemma":0.001972147,"teacher_disagreement_score":0.0016288131,"about_ca_system_score_codex":0.00017219286,"about_ca_system_score_gemma":0.0000725053,"threshold_uncertainty_score":0.003867209},"labels":[],"label_agreement":null},{"id":"W2122449290","doi":"10.1086/516710","title":"Discovery of the Widest Very Low Mass Binary","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Low Mass; Binary number; Spectral line; Binary star; Binary system; Mass spectrum; Mass distribution; Stellar classification; X-ray binary","score_opus":0.007447027824865743,"score_gpt":0.21460623763147593,"score_spread":0.20715920980661018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122449290","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99476284,0.001512911,0.00095709646,0.00023046049,0.000042125277,0.000005067996,0.00008776129,0.000029748993,0.00237211],"genre_scores_gemma":[0.99849224,0.00013972801,0.0006977233,0.00012625878,0.000041126095,0.0000030065303,0.00015493439,0.0000035913963,0.0003413708],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99984086,0.000016855134,0.000010949389,0.00005925758,0.000039614424,0.00003247645],"domain_scores_gemma":[0.999617,0.00009009116,0.00010114424,0.00004640128,0.000036399597,0.000108933615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023791369,0.00012468666,0.00032736702,0.0008588057,0.0008579632,0.0014225398,0.00033268324,0.00080392114,0.0010290385],"category_scores_gemma":[0.0009747708,0.0001973797,0.000096662865,0.00031961533,0.00047388097,0.00044087326,0.0010350745,0.00070011406,0.00057468296],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068035047,0.00020068817,0.4022846,0.00022540406,0.000086282234,0.011455855,0.0013552461,0.0003154069,0.46989697,0.007849093,0.0031035903,0.102546535],"study_design_scores_gemma":[0.000053250238,0.0009616172,0.77112806,0.000065932974,0.0001320102,0.11598139,0.0005271663,0.0019375663,0.071791306,0.0061769714,0.031162998,0.00008174748],"about_ca_topic_score_codex":0.00019064968,"about_ca_topic_score_gemma":0.00020566414,"teacher_disagreement_score":0.0014225398,"about_ca_system_score_codex":0.00021870848,"about_ca_system_score_gemma":0.0001057431,"threshold_uncertainty_score":0.0034425259},"labels":[],"label_agreement":null},{"id":"W2122450362","doi":"10.1088/0004-637x/777/1/14","title":"H I SHELLS AND SUPERSHELLS IN THE I-GALFA H I 21 cm LINE SURVEY. I. FAST-EXPANDING H I SHELLS ASSOCIATED WITH SUPERNOVA REMNANTS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Supernova; Line (geometry); Astronomy; Galactic plane; Shell (structure); Galaxy; Supernova remnant; Longitude; Hydrogen line; Latitude","score_opus":0.014497689092305347,"score_gpt":0.22657608492381673,"score_spread":0.2120783958315114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122450362","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99879104,0.00013837405,0.000070975926,0.000015630587,0.0000011224289,0.0000038029916,0.0002815131,0.000007866841,0.0006898844],"genre_scores_gemma":[0.9983664,0.00014489796,0.00027291197,0.00002235699,0.0000045654274,0.000004897526,0.00094640267,0.0000032349192,0.00023432303],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998672,0.00002053282,0.000011603732,0.0000326355,0.000023144154,0.00004495743],"domain_scores_gemma":[0.999584,0.000048252154,0.00020852596,0.000032896638,0.000036621936,0.000089709676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019158486,0.00013659903,0.000112126494,0.001151751,0.00024450565,0.0003742035,0.0002516943,0.00021505744,0.0005881514],"category_scores_gemma":[0.00047920243,0.000114782015,0.00015155466,0.0006963282,0.0002432229,0.0002647654,0.0005288732,0.00013077317,0.00019452153],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040049552,0.000011849864,0.99360317,0.0000082282,0.000017656734,0.00007830515,0.00013836181,0.00006741004,0.003026738,0.00004885336,0.00014978123,0.002809517],"study_design_scores_gemma":[7.7395373e-7,0.0000072131306,0.9993944,0.0000017810266,0.000003433464,0.00007973619,0.00007685909,0.000062781495,0.00013498843,0.00000933428,0.00022761199,0.0000010723775],"about_ca_topic_score_codex":0.013776796,"about_ca_topic_score_gemma":0.031174997,"teacher_disagreement_score":0.013776796,"about_ca_system_score_codex":0.0002512656,"about_ca_system_score_gemma":0.00011792572,"threshold_uncertainty_score":0.027393222},"labels":[],"label_agreement":null},{"id":"W2122463823","doi":"10.1088/0004-637x/732/2/90","title":"ACCRETION OF A TERRESTRIAL-LIKE MINOR PLANET BY A WHITE DWARF","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Planet; Accretion (finance); Dwarf planet; Parent body; Infrared; Debris; Mantle (geology); Spectroscopy","score_opus":0.016815580991834986,"score_gpt":0.21607620676827063,"score_spread":0.19926062577643566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122463823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937797,0.000043908694,0.000098407334,0.000006290515,0.0000013551025,0.0000013975928,0.00003137908,0.0000087902845,0.0004305259],"genre_scores_gemma":[0.99922514,0.000039156304,0.00021944188,0.000011289443,0.000004536031,0.0000012992118,0.00015787999,0.000003495396,0.00033764716],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999658,0.00000274204,0.0000018003121,0.000012186455,0.000008134746,0.000009448745],"domain_scores_gemma":[0.9998957,0.000011010987,0.000043513388,0.000015886639,0.000007925587,0.00002608443],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007712683,0.00028351118,0.00021911108,0.0006073065,0.00037549908,0.0004939474,0.0002376874,0.00021114663,0.00046304252],"category_scores_gemma":[0.0001610329,0.00010245937,0.00012569525,0.00035075797,0.0002393473,0.00021354339,0.0004893438,0.00011405232,0.00023046718],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053133164,0.00012507186,0.4901769,0.00008417044,0.00013543964,0.004300178,0.00051073305,0.001347749,0.48697817,0.00082200917,0.00031969955,0.0146685615],"study_design_scores_gemma":[0.000027826532,0.00047196978,0.9348271,0.000008237055,0.0000615471,0.0023098683,0.00048293627,0.004277718,0.053535663,0.00048270606,0.0035004162,0.0000139563435],"about_ca_topic_score_codex":0.0011821362,"about_ca_topic_score_gemma":0.0018375228,"teacher_disagreement_score":0.0011821362,"about_ca_system_score_codex":0.00021525644,"about_ca_system_score_gemma":0.000078192636,"threshold_uncertainty_score":0.0023505092},"labels":[],"label_agreement":null},{"id":"W2122522097","doi":"10.1088/0004-637x/691/2/1042","title":"NEAR-INFRARED [Fe II] AND H<sub>2</sub>LINE OBSERVATIONS OF THE SUPERNOVA REMNANT 3C 396: PROBING THE PRESUPERNOVA CIRCUMSTELLAR MATERIALS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Supernova remnant; Supernova; Line (geometry); Red supergiant; Emission spectrum; Telescope; Astronomy; Infrared; Spectral line; Supergiant; Stars","score_opus":0.014757020401035496,"score_gpt":0.21143626279042177,"score_spread":0.19667924238938628,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122522097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918634,0.000038331236,0.000081218226,0.000009946791,0.0000014945699,0.0000036353586,0.00015107417,0.000015214127,0.0005127],"genre_scores_gemma":[0.9979761,0.00006692142,0.0007446224,0.000021209727,0.0000078724415,0.0000067538117,0.0008795125,0.000015467356,0.00028142452],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993634,0.0000035095218,0.000003439581,0.000016344944,0.000024067891,0.000016207],"domain_scores_gemma":[0.99982494,0.000008347887,0.000047443074,0.00001744398,0.000025359985,0.000076475946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016187069,0.00033108096,0.00023015533,0.00049998926,0.0006083313,0.00028715262,0.00030656735,0.00035693237,0.0010144685],"category_scores_gemma":[0.00014777321,0.00017445764,0.00029298765,0.000273646,0.00019039371,0.00017969958,0.00046307326,0.00030542753,0.0004302549],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078591076,0.00014057076,0.25526336,0.00005780594,0.00008484494,0.0019599646,0.00037698165,0.00044501506,0.734468,0.0001782548,0.00032609628,0.005913243],"study_design_scores_gemma":[0.000032704156,0.00017663806,0.9737307,0.000008026216,0.00002715239,0.0017853292,0.00016686684,0.0009166712,0.021522352,0.00011657384,0.0015022922,0.000014688938],"about_ca_topic_score_codex":0.004810371,"about_ca_topic_score_gemma":0.009490311,"teacher_disagreement_score":0.004810371,"about_ca_system_score_codex":0.00022765486,"about_ca_system_score_gemma":0.00012080978,"threshold_uncertainty_score":0.009564698},"labels":[],"label_agreement":null},{"id":"W2122624438","doi":"10.1088/0004-637x/780/1/112","title":"THE UNUSUAL SMOOTHNESS OF THE EXTRAGALACTIC UNRESOLVED RADIO BACKGROUND","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Cosmic infrared background; COSMIC cancer database; Astronomy; Halo; Cosmic microwave background; Dark matter; Cosmology; Galaxy cluster; Universe; Background radiation; Anisotropy","score_opus":0.009932598697462795,"score_gpt":0.21568374260046705,"score_spread":0.20575114390300425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122624438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94698274,0.0010034168,0.03483198,0.0004766643,0.00005069374,0.000017291188,0.0015612782,0.0005296094,0.014546276],"genre_scores_gemma":[0.9957955,0.00021368818,0.0025573175,0.000048693448,0.000056837376,0.0000030185254,0.0006277911,0.00004581783,0.0006513111],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998404,0.000016744321,0.000006901628,0.00006393383,0.000044680834,0.000027347667],"domain_scores_gemma":[0.99867284,0.00035279556,0.00032975612,0.00039584094,0.00014217735,0.0001066406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028073,0.00015492756,0.00019320894,0.0007744605,0.00019171169,0.00093772326,0.00039655535,0.00025538428,0.0016246182],"category_scores_gemma":[0.0019405105,0.00022525585,0.00013743166,0.0008395731,0.00035018727,0.00057219906,0.0004515854,0.0005758165,0.0005372986],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005138311,0.000096109274,0.6674308,0.00026011348,0.0002534394,0.0023873511,0.0011613957,0.011426166,0.14685322,0.038439076,0.0062401765,0.12493833],"study_design_scores_gemma":[0.000008801087,0.00002733634,0.9777215,0.000016141857,0.00004759247,0.001512539,0.00015648518,0.0043379418,0.003175485,0.0064962297,0.006473443,0.000026367163],"about_ca_topic_score_codex":0.0017459888,"about_ca_topic_score_gemma":0.0019243658,"teacher_disagreement_score":0.0017459888,"about_ca_system_score_codex":0.00019123027,"about_ca_system_score_gemma":0.00007111035,"threshold_uncertainty_score":0.0054348707},"labels":[],"label_agreement":null},{"id":"W2122672163","doi":"10.1088/0004-637x/795/1/62","title":"CHANGING IONIZATION CONDITIONS IN SDSS GALAXIES WITH ACTIVE GALACTIC NUCLEI AS A FUNCTION OF ENVIRONMENT FROM PAIRS TO CLUSTERS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University; University of Victoria","funders":"","keywords":"Active galactic nucleus; Galaxy; Accretion (finance); Ionization; Quasar; Galaxy cluster; Radio galaxy; Function (biology)","score_opus":0.004455734640374884,"score_gpt":0.18426583925723256,"score_spread":0.17981010461685767,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122672163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997272,0.000026873027,0.000029656305,0.0000024403068,2.7258963e-7,7.2497477e-7,0.000089478475,0.0000031869336,0.00012015639],"genre_scores_gemma":[0.99960226,0.000016402839,0.000046976482,0.0000034875168,0.0000012016864,0.0000011498624,0.00025818223,0.0000020673713,0.00006824792],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979466,0.000038064918,0.000014800636,0.000066851455,0.000033168657,0.000052554136],"domain_scores_gemma":[0.99868506,0.00021923274,0.0005365663,0.00013349333,0.0001206679,0.0003048983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003485928,0.00026484442,0.0003065197,0.0015404974,0.00030350478,0.0006051957,0.00023446487,0.00019896845,0.0009150805],"category_scores_gemma":[0.001166294,0.000154409,0.00024768634,0.001338479,0.0005324193,0.00037872852,0.00085274095,0.00016117377,0.00029823158],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007445393,0.000014105831,0.995771,0.0000043247665,0.000034733297,0.00002838577,0.00016221928,0.00016976781,0.00248867,0.000026760505,0.00003420492,0.001191351],"study_design_scores_gemma":[0.0000011370292,0.000012858618,0.9995617,4.1362864e-7,0.0000053286026,0.000025627249,0.00008806314,0.00010618715,0.00014968892,0.000013084026,0.000034734036,0.0000012852358],"about_ca_topic_score_codex":0.007971963,"about_ca_topic_score_gemma":0.010235401,"teacher_disagreement_score":0.007971963,"about_ca_system_score_codex":0.00034332325,"about_ca_system_score_gemma":0.00011130336,"threshold_uncertainty_score":0.01585114},"labels":[],"label_agreement":null},{"id":"W2122990195","doi":"10.1086/499776","title":"A Neutron Star with a Massive Progenitor in Westerlund 1","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"High-pressure geophysics and materials","field":"Earth and Planetary Sciences","cited_by":259,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Pulsar; Physics; Astrophysics; Neutron star; Magnetar; Binary pulsar; Astronomy; X-ray pulsar; Luminosity; RADIUS; Pulsar planet; Millisecond pulsar; Galaxy","score_opus":0.006666263875062734,"score_gpt":0.1946818980923481,"score_spread":0.18801563421728537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2122990195","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99914944,0.0001743631,0.00006760066,0.000020843003,0.000013780851,0.000003564471,0.000031765114,0.000005400304,0.00053325854],"genre_scores_gemma":[0.9981336,0.00024515577,0.00025094266,0.00003932298,0.000012442808,0.000002257518,0.00023635586,0.0000028100437,0.0010771912],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985933,0.0000060772036,0.000010291204,0.000046794747,0.000037268983,0.000040175888],"domain_scores_gemma":[0.9997608,0.000011623274,0.000087007786,0.000014275985,0.0000127860285,0.000113563554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016907573,0.0004075009,0.0004737331,0.00072488864,0.0012864837,0.0008955098,0.00050940143,0.0005591721,0.0008432645],"category_scores_gemma":[0.00043981484,0.0002864485,0.00018231253,0.000490867,0.00037582498,0.000525002,0.0010943256,0.0004055825,0.00035975635],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011091167,0.0003804526,0.86148345,0.00010543102,0.000100768135,0.047921065,0.002262392,0.00057995325,0.06562641,0.0017502478,0.00081572664,0.017864978],"study_design_scores_gemma":[0.00007343003,0.0017626964,0.89754295,0.000046023964,0.00010226222,0.06032712,0.00156696,0.0012498155,0.014629253,0.0007605562,0.021884797,0.00005409498],"about_ca_topic_score_codex":0.005421752,"about_ca_topic_score_gemma":0.012088723,"teacher_disagreement_score":0.005421752,"about_ca_system_score_codex":0.00077661703,"about_ca_system_score_gemma":0.00035061585,"threshold_uncertainty_score":0.010780394},"labels":[],"label_agreement":null},{"id":"W2123139451","doi":"10.1086/505646","title":"Black Hole Masses and Eddington Ratios at 0.3 &lt;<i>z</i>&lt; 4","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":428,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Redshift; Eddington luminosity; Active galactic nucleus; Luminosity; Galaxy; Black hole (networking); Supermassive black hole; Astronomy","score_opus":0.005367865110753353,"score_gpt":0.1998967449256276,"score_spread":0.19452887981487424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123139451","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983859,0.000056275858,0.000095241645,0.00002927114,0.0000017200075,0.0000021861886,0.0006118701,0.00001456676,0.0008029564],"genre_scores_gemma":[0.99845946,0.000026645888,0.00005878692,0.0000075293483,0.00000517259,0.0000019212666,0.00069814624,0.0000051244133,0.0007374175],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998783,0.000012913711,0.0000051831726,0.000020731999,0.0000149994075,0.000067896486],"domain_scores_gemma":[0.9981858,0.00029466927,0.0009291863,0.0000872901,0.00013416974,0.0003687925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036543023,0.00021696235,0.00016113903,0.0016895039,0.00025482487,0.0006469205,0.00033246382,0.00037336256,0.0026518435],"category_scores_gemma":[0.0013893249,0.00017523939,0.00020714724,0.00066454103,0.00032883967,0.0005169989,0.00037759705,0.00037370244,0.0007732021],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002492646,0.000057247973,0.9927779,0.0000052225255,0.00003207922,0.00012000118,0.00022314483,0.0004909818,0.0014388406,0.00047240165,0.0005432272,0.0035897696],"study_design_scores_gemma":[0.000004092708,0.000035292705,0.9977307,0.0000020464777,0.000007695271,0.00010499232,0.000107705935,0.0010779075,0.00047564707,0.00017484384,0.0002742429,0.000004788786],"about_ca_topic_score_codex":0.0042190645,"about_ca_topic_score_gemma":0.005698678,"teacher_disagreement_score":0.0042190645,"about_ca_system_score_codex":0.0003447789,"about_ca_system_score_gemma":0.000074717434,"threshold_uncertainty_score":0.008871317},"labels":[],"label_agreement":null},{"id":"W2123157963","doi":"10.1088/0004-637x/797/2/128","title":"GLOBULAR CLUSTER SYSTEMS IN BRIGHTEST CLUSTER GALAXIES: A NEAR-UNIVERSAL LUMINOSITY FUNCTION?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Astrophysics; Physics; Globular cluster; Luminosity function; Galaxy; Luminosity; Galaxy cluster; Astronomy; Halo; Cluster (spacecraft)","score_opus":0.0051575197417157125,"score_gpt":0.18962501361560644,"score_spread":0.18446749387389072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123157963","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937831,0.0006998941,0.0004314578,0.0005357558,0.000009320705,0.000005798351,0.00047270322,0.000037642738,0.00402426],"genre_scores_gemma":[0.99926525,0.00007165985,0.00006148894,0.00003592801,0.000008323473,0.000002030284,0.0001921798,0.000006403489,0.00035678092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969065,0.000051626783,0.000011991395,0.000097839235,0.00003086138,0.000117025666],"domain_scores_gemma":[0.9974649,0.0005072742,0.00067895907,0.00026358836,0.0003409584,0.00074435875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006703406,0.00020770678,0.0002888049,0.0019455798,0.0007294933,0.0018130394,0.00060537976,0.0008172277,0.0089793885],"category_scores_gemma":[0.0042961966,0.00017349682,0.00022238286,0.0012693204,0.0009625055,0.0014541016,0.0010755248,0.00036408246,0.00095270947],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079103054,0.000033588833,0.9855085,0.000014636041,0.000023327246,0.00005582462,0.00039228116,0.00013805793,0.0007389952,0.0020678034,0.00095503987,0.009992899],"study_design_scores_gemma":[0.0000039206107,0.000015368225,0.9959319,0.000011832774,0.00001477367,0.00016625438,0.00072102237,0.00058908237,0.0001059031,0.0017654035,0.0006697851,0.0000047495528],"about_ca_topic_score_codex":0.020511653,"about_ca_topic_score_gemma":0.022522407,"teacher_disagreement_score":0.020511653,"about_ca_system_score_codex":0.0007848638,"about_ca_system_score_gemma":0.00055546855,"threshold_uncertainty_score":0.040784538},"labels":[],"label_agreement":null},{"id":"W2123196553","doi":"10.1088/0004-637x/790/1/19","title":"THE INFLUENCE OF THERMAL PRESSURE ON EQUILIBRIUM MODELS OF HYPERMASSIVE NEUTRON STAR MERGER REMNANTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Neutron star; Compact star; Baryon; Gravitational collapse; Thermal equilibrium; Equation of state; Angular momentum; Instability; Gravitational energy","score_opus":0.011034399623164779,"score_gpt":0.2819658070206646,"score_spread":0.2709314073974998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123196553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955319,0.00008872117,0.0028872523,0.000039051,0.000004514402,0.0000070901324,0.00006130158,0.00004635714,0.0013338645],"genre_scores_gemma":[0.9985802,0.00006388919,0.0010166868,0.000010293223,0.000004782317,0.000009666314,0.00010850064,0.0000197199,0.00018630471],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998586,0.00005735514,0.000007771922,0.000021634034,0.000017722861,0.00003686315],"domain_scores_gemma":[0.99933535,0.0002731427,0.0001487316,0.00005244255,0.00007210899,0.0001183117],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053845195,0.0005328803,0.0005050231,0.00065122696,0.00070476957,0.0012212202,0.0011063004,0.00057117897,0.0011258905],"category_scores_gemma":[0.0029684205,0.00045054295,0.00060211105,0.00031127987,0.0011367486,0.0009593835,0.00084185146,0.00039728204,0.0001599682],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001236334,0.000048859103,0.010484364,0.000021492277,0.00004018634,0.00013453134,0.00007505226,0.98085576,0.0014705533,0.0057146084,0.00008699899,0.0009439851],"study_design_scores_gemma":[0.00001938218,0.000035939745,0.0016965568,0.0000036270899,0.00000818282,0.000017815964,0.000036836376,0.99561775,0.00028192258,0.0022134995,0.00006224613,0.000006258521],"about_ca_topic_score_codex":0.014088192,"about_ca_topic_score_gemma":0.00884689,"teacher_disagreement_score":0.014088192,"about_ca_system_score_codex":0.0010124355,"about_ca_system_score_gemma":0.0005082948,"threshold_uncertainty_score":0.028012335},"labels":[],"label_agreement":null},{"id":"W2123217226","doi":"10.1086/505634","title":"Further Observations and Analysis of the Rapidly Pulsating Subdwarf B Star EC 20117−4014","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Subdwarf; Physics; Surface gravity; Astrophysics; Stars; Effective temperature; Logarithm","score_opus":0.012838809566126125,"score_gpt":0.21418796775297355,"score_spread":0.20134915818684743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123217226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93604493,0.0007121178,0.0054046265,0.0011060012,0.00014958608,0.00025637148,0.006848475,0.00032422302,0.049153686],"genre_scores_gemma":[0.914262,0.0005808435,0.015746798,0.0015178529,0.00014691906,0.00015975985,0.028011799,0.0002015317,0.03937257],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997974,0.00001824548,0.000010012584,0.000052471798,0.000057320623,0.00006451348],"domain_scores_gemma":[0.99883944,0.00017472559,0.00015579176,0.00016581162,0.000333915,0.0003303847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008913513,0.0004308024,0.0004973346,0.0017066792,0.0017030524,0.0009998541,0.0005339142,0.0010408206,0.008900819],"category_scores_gemma":[0.0005679451,0.0002517447,0.0007824547,0.0015166532,0.00018475128,0.0005665851,0.0007005228,0.0008769981,0.002639725],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025800676,0.001024935,0.33057305,0.000373232,0.00032870017,0.002335358,0.0005417231,0.0022839871,0.54951864,0.0022991274,0.015739156,0.09240186],"study_design_scores_gemma":[0.00008430253,0.0006051272,0.95396745,0.000030570984,0.000082442144,0.0007554466,0.00048665114,0.0016665919,0.017354565,0.0009026586,0.024026547,0.000037655347],"about_ca_topic_score_codex":0.009975202,"about_ca_topic_score_gemma":0.016997933,"teacher_disagreement_score":0.009975202,"about_ca_system_score_codex":0.0006474887,"about_ca_system_score_gemma":0.0008414063,"threshold_uncertainty_score":0.029776216},"labels":[],"label_agreement":null},{"id":"W2123225501","doi":"10.1088/0004-637x/707/2/1766","title":"BLAST: CORRELATIONS IN THE COSMIC FAR-INFRARED BACKGROUND AT 250, 350, AND 500 μm REVEAL CLUSTERING OF STAR-FORMING GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Halo; Redshift; Dark matter; Context (archaeology); Star formation; RADIUS; Spectral density; Astronomy; Statistics","score_opus":0.011657194334759435,"score_gpt":0.22486063657934313,"score_spread":0.2132034422445837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123225501","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9697804,0.00007321751,0.0020293123,0.00010523452,0.000012387074,0.000009300265,0.022756793,0.0014943089,0.0037390266],"genre_scores_gemma":[0.9782601,0.000029982879,0.0021719579,0.000036106085,0.0000145307895,0.000009644918,0.017993594,0.00018745073,0.0012965889],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998572,0.00001704865,0.0000054026964,0.000046159013,0.00003559169,0.000038543658],"domain_scores_gemma":[0.9992514,0.00018390719,0.00013992738,0.00010563168,0.000074083895,0.000244897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002687192,0.0002755898,0.00030497188,0.00091831473,0.00034441127,0.00047582688,0.00028164123,0.00028806188,0.009398062],"category_scores_gemma":[0.00062908075,0.00021511364,0.00033389035,0.0012082706,0.00020692043,0.00029016528,0.00038507354,0.00033339064,0.0012344379],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003009611,0.00029626786,0.69339365,0.00019722637,0.0005069578,0.00073076104,0.0005591025,0.009408933,0.18257587,0.0042428277,0.06472204,0.0403567],"study_design_scores_gemma":[0.00004081027,0.000050152274,0.9850846,0.0000033023123,0.000039489238,0.00015278078,0.000074939126,0.0045099077,0.007828219,0.00064130104,0.0015592646,0.00001524881],"about_ca_topic_score_codex":0.004607971,"about_ca_topic_score_gemma":0.009065406,"teacher_disagreement_score":0.009398062,"about_ca_system_score_codex":0.00016347125,"about_ca_system_score_gemma":0.00014628028,"threshold_uncertainty_score":0.031439662},"labels":[],"label_agreement":null},{"id":"W2123494985","doi":"10.1086/506469","title":"A Panoramic Mid‐Infrared Survey of Two Distant Clusters","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Canadian Space Agency; National Aeronautics and Space Administration; California Institute of Technology; Ames Research Center","keywords":"Astrophysics; Physics; Infrared; Galaxy; Population; Star formation; Luminous infrared galaxy; Cluster (spacecraft); Astronomy; Active galactic nucleus; Medicine","score_opus":0.008183427528281832,"score_gpt":0.21819889487269362,"score_spread":0.2100154673444118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123494985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.987978,0.00017072745,0.00023186159,0.00005169428,0.0000060242664,0.000029409546,0.0054490077,0.0000867288,0.0059965933],"genre_scores_gemma":[0.9637025,0.00021047548,0.0017629376,0.00006349159,0.00003214022,0.00006761095,0.02753137,0.000020292246,0.006609122],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998667,0.000011224815,0.0000064916744,0.00004034632,0.000036375583,0.000038899638],"domain_scores_gemma":[0.99967813,0.000012494574,0.000067745204,0.00002640489,0.000055493983,0.00015970571],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011796373,0.00020498344,0.00014428725,0.0018392762,0.00044821025,0.00039708096,0.00026030603,0.00018736995,0.00466681],"category_scores_gemma":[0.00021624178,0.000153089,0.00013472015,0.0012555071,0.00008785919,0.00023015599,0.0008194853,0.0001599473,0.0010691864],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004717063,0.00012427977,0.91537726,0.00011059007,0.00009895736,0.0004279108,0.00090455124,0.0003319766,0.03211562,0.00048194057,0.010269792,0.039285503],"study_design_scores_gemma":[0.000007872931,0.000021120275,0.99411976,0.0000031419981,0.0000065067716,0.000111042384,0.000107354004,0.000077322344,0.00021481216,0.000013180291,0.005315405,0.0000024686701],"about_ca_topic_score_codex":0.01785016,"about_ca_topic_score_gemma":0.038506467,"teacher_disagreement_score":0.01785016,"about_ca_system_score_codex":0.00031090557,"about_ca_system_score_gemma":0.00027836728,"threshold_uncertainty_score":0.03549254},"labels":[],"label_agreement":null},{"id":"W2123624806","doi":"10.1088/0004-637x/812/1/48","title":"TESTS OF THE PLANETARY HYPOTHESIS FOR PTFO 8-8695b","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomical and nuclear sciences","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"Fonds De La Recherche Scientifique - FNRS; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Physics; Astronomy; Astrophysics; Astrobiology","score_opus":0.02565544231307992,"score_gpt":0.22357446107614812,"score_spread":0.1979190187630682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123624806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99335855,0.00035938495,0.0007679139,0.0005400765,0.000045187608,0.000015358657,0.00023846091,0.000044737462,0.0046302387],"genre_scores_gemma":[0.999102,0.00005391621,0.0002449627,0.000111378264,0.000041642248,0.00000858572,0.00024081534,0.000009165891,0.00018746509],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990854,0.00014832108,0.00010685877,0.00026749275,0.0002107742,0.0001811112],"domain_scores_gemma":[0.98868424,0.0054009617,0.002410135,0.0013553209,0.00048560862,0.0016638205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002182624,0.00044791683,0.00067305675,0.0016012508,0.0013141913,0.0013664601,0.001577806,0.0017621306,0.008761375],"category_scores_gemma":[0.0098169055,0.00023385584,0.0005844407,0.0008257035,0.002142141,0.0015448299,0.0018135476,0.00078415615,0.0011175893],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.005331857,0.00036253082,0.88605267,0.0003289536,0.00038590212,0.0064711184,0.0021183062,0.0018377671,0.057403684,0.0078023723,0.0014134491,0.030491428],"study_design_scores_gemma":[0.00042435946,0.001570387,0.94789153,0.00014627869,0.00017833694,0.0105055375,0.0025094952,0.011414393,0.008442136,0.009840468,0.0069920025,0.00008497734],"about_ca_topic_score_codex":0.00089800527,"about_ca_topic_score_gemma":0.0004839607,"teacher_disagreement_score":0.008761375,"about_ca_system_score_codex":0.0004599673,"about_ca_system_score_gemma":0.00022453385,"threshold_uncertainty_score":0.02930975},"labels":[],"label_agreement":null},{"id":"W2123808593","doi":"10.1088/0004-637x/768/2/159","title":"MISALIGNMENT OF MAGNETIC FIELDS AND OUTFLOWS IN PROTOSTELLAR CORES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":168,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; National Research Council Canada; Western University; University of Manitoba","funders":"","keywords":"Protostar; Physics; Astrophysics; Magnetic field; Circumstellar disk; Polarization (electrochemistry); Star formation; Perpendicular; Low Mass; Stars; Geometry","score_opus":0.007177028126291354,"score_gpt":0.2167922688171028,"score_spread":0.20961524069081144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2123808593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999622,0.000017900793,0.0000931471,0.00000528047,6.8934537e-7,0.0000010499541,0.00005633785,0.0000057338802,0.00019788586],"genre_scores_gemma":[0.9996779,0.000011183752,0.00015049607,0.000004900145,0.000002294596,0.0000013888856,0.00009619594,0.0000017945664,0.00005389227],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990773,0.000013492972,0.0000061920427,0.000034207074,0.000016071126,0.000022239978],"domain_scores_gemma":[0.99941194,0.000104949024,0.00023624883,0.00005688549,0.000075641554,0.00011437132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015836931,0.00012867896,0.00018201067,0.00047350235,0.00034037646,0.00041549813,0.00014805981,0.00023158813,0.00044170913],"category_scores_gemma":[0.0009264453,0.0001492327,0.00010763493,0.00030886324,0.00028115296,0.00019943094,0.00030801224,0.00019376812,0.000099357734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034637016,0.000043190175,0.9304016,0.0000238976,0.00003377567,0.00017176435,0.00029614603,0.0010562983,0.062833466,0.00011519215,0.0001070476,0.0045712884],"study_design_scores_gemma":[0.000007335907,0.00002917609,0.9952655,0.0000021107394,0.000010022522,0.000108034714,0.000063096006,0.00073267764,0.0035831225,0.00004919948,0.00014657927,0.0000032221233],"about_ca_topic_score_codex":0.0026422888,"about_ca_topic_score_gemma":0.004114333,"teacher_disagreement_score":0.0026422888,"about_ca_system_score_codex":0.00028904455,"about_ca_system_score_gemma":0.00012685468,"threshold_uncertainty_score":0.005253792},"labels":[],"label_agreement":null},{"id":"W2124079745","doi":"10.1088/0004-637x/721/1/137","title":"THE BOLOCAM GALACTIC PLANE SURVEY: λ = 1.1 AND 0.35 mm DUST CONTINUUM EMISSION IN THE GALACTIC CENTER REGION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Galaxy; Galactic Center; Astronomy; Supernova; Star formation; Spitzer Space Telescope; Infrared; Molecular cloud; Telescope; Stars","score_opus":0.011862425211988936,"score_gpt":0.24198782192462315,"score_spread":0.2301253967126342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124079745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9715092,0.0013459958,0.00020482132,0.0001434798,0.000016536953,0.000026159805,0.01935038,0.00012954856,0.007273693],"genre_scores_gemma":[0.9645403,0.0009410879,0.000853728,0.000100836354,0.000037934595,0.000025190488,0.03145975,0.0000427868,0.0019984392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998603,0.000013059097,0.00000608016,0.000041901643,0.00004261954,0.00003604137],"domain_scores_gemma":[0.9997271,0.000012402394,0.00012433095,0.00001673786,0.000047738875,0.00007170808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018791851,0.0002487888,0.00017972049,0.0021787144,0.00022691244,0.00061572855,0.00024477622,0.00019893714,0.0017639071],"category_scores_gemma":[0.00024702883,0.00012433498,0.00017371334,0.0016528765,0.00012645179,0.00015519961,0.00033644354,0.00024351898,0.0007328217],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015781562,0.000036856403,0.97078615,0.00008348673,0.000119096636,0.00014898997,0.00028002332,0.00022434167,0.011325921,0.00017831476,0.0067295255,0.009929365],"study_design_scores_gemma":[0.0000031535642,0.0000033926085,0.99868935,0.0000037014756,0.0000039882584,0.000019673815,0.000018288674,0.000020304738,0.00007047836,0.0000038143066,0.0011632795,5.88492e-7],"about_ca_topic_score_codex":0.056493044,"about_ca_topic_score_gemma":0.08290624,"teacher_disagreement_score":0.056493044,"about_ca_system_score_codex":0.0009438346,"about_ca_system_score_gemma":0.0002425881,"threshold_uncertainty_score":0.11232841},"labels":[],"label_agreement":null},{"id":"W2124149528","doi":"10.1088/0004-637x/714/1/894","title":"DISCOVERY OF A SECOND TRANSIENT LOW-MASS X-RAY BINARY IN THE GLOBULAR CLUSTER NGC 6440","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Globular cluster; Neutron star; Luminosity; Erg; Wide Field Camera 3; Astronomy; Millisecond pulsar; Galaxy; Hubble space telescope; Optics","score_opus":0.006759545080613844,"score_gpt":0.2159266419656351,"score_spread":0.20916709688502125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124149528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99710184,0.00013691542,0.00031995555,0.00020219394,0.000031864056,0.000010357478,0.00014603413,0.000045625915,0.0020052022],"genre_scores_gemma":[0.9982948,0.00002475854,0.00018523732,0.00008823826,0.000018659091,0.000004309575,0.00020655851,0.0000067030473,0.0011707672],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999866,0.0000056109934,0.0000043244013,0.000049376533,0.000021291904,0.000053306343],"domain_scores_gemma":[0.9994925,0.00007747882,0.00007964552,0.000063043444,0.00004665996,0.00024060524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033327402,0.00028162537,0.00053503417,0.001026724,0.0022004135,0.0015891539,0.00058887055,0.001658722,0.0033350363],"category_scores_gemma":[0.00042701085,0.00031911992,0.00039620622,0.0006316072,0.00050217565,0.0003591659,0.0011929736,0.00063913624,0.00073720864],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025081038,0.00051347865,0.44688794,0.00024091589,0.00024329775,0.023516947,0.002179436,0.001425802,0.48733306,0.005282483,0.003962053,0.025906498],"study_design_scores_gemma":[0.00011313448,0.0008440778,0.9659435,0.00001980599,0.00011943425,0.0052536717,0.0009369323,0.0031548133,0.016255843,0.001313983,0.0059983423,0.000046427376],"about_ca_topic_score_codex":0.0049542016,"about_ca_topic_score_gemma":0.0048957276,"teacher_disagreement_score":0.0049542016,"about_ca_system_score_codex":0.001012153,"about_ca_system_score_gemma":0.0004236014,"threshold_uncertainty_score":0.011156797},"labels":[],"label_agreement":null},{"id":"W2124307771","doi":"10.1088/0004-637x/812/1/19","title":"ON THE EVOLUTION OF MAGNETIC WHITE DWARFS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Convection; Photosphere; Magnetohydrodynamics; Radiative transfer; Magnetic field; Radiative cooling; Magnetism","score_opus":0.013200848951622848,"score_gpt":0.21441931111060672,"score_spread":0.20121846215898387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124307771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99448293,0.00014484314,0.0017986972,0.00015328248,0.000019057792,0.000016531805,0.00013074461,0.00007125123,0.0031826166],"genre_scores_gemma":[0.998055,0.000073978255,0.0010451836,0.0000428019,0.0000109878565,0.000013343627,0.00016610857,0.000035103978,0.00055749825],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99991107,0.00002599399,0.0000028202153,0.00001262858,0.000015163925,0.00003224237],"domain_scores_gemma":[0.9996208,0.00015578372,0.000048625203,0.000023536226,0.00004915509,0.00010216837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034770297,0.00046021488,0.00067309977,0.00036546384,0.00069349934,0.00080818444,0.0005628089,0.00074048096,0.0010027627],"category_scores_gemma":[0.001800536,0.00027375063,0.0005407254,0.0002618119,0.00077285,0.00047769787,0.00069366494,0.0005302949,0.00014001674],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028621353,0.000104219835,0.029337617,0.00005773223,0.000119795666,0.00033665393,0.00024211487,0.9519328,0.009588902,0.004279671,0.00053347397,0.0031808408],"study_design_scores_gemma":[0.00014226604,0.00012384605,0.010707869,0.000009913964,0.00002854164,0.000050481263,0.0001082592,0.9844657,0.001402757,0.001729742,0.0012157334,0.00001490599],"about_ca_topic_score_codex":0.0131586315,"about_ca_topic_score_gemma":0.0064668097,"teacher_disagreement_score":0.0131586315,"about_ca_system_score_codex":0.0008522414,"about_ca_system_score_gemma":0.0007009035,"threshold_uncertainty_score":0.026164055},"labels":[],"label_agreement":null},{"id":"W2124391162","doi":"10.1086/519791","title":"Polarization Shadows of Extragalactic Sources by the Local Magnetoionic Interstellar Medium","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Polarization (electrochemistry); Astrophysics; Sky; Interstellar medium; Depolarization; Astronomy; Galaxy; Optics","score_opus":0.0049749365941632005,"score_gpt":0.2016049425393569,"score_spread":0.1966300059451937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124391162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999141,0.000103512444,0.0001322077,0.000007852265,7.8540586e-7,7.591057e-7,0.00015547404,0.000009146549,0.00044931355],"genre_scores_gemma":[0.9995153,0.000045796714,0.00004897071,0.0000032019364,0.0000033688045,6.393304e-7,0.00031524512,0.0000021170167,0.00006541797],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998746,0.000021534403,0.000007643085,0.00002277638,0.000037337788,0.00003609007],"domain_scores_gemma":[0.99888355,0.00032537247,0.00041528078,0.00013458684,0.00009955158,0.0001415773],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016815562,0.00013315488,0.00016150514,0.00082074746,0.00018781677,0.00038853087,0.00010112868,0.0001221697,0.00089948584],"category_scores_gemma":[0.0010467048,0.00012016924,0.00013288244,0.000838469,0.00029525338,0.00030234235,0.00071253866,0.00013799501,0.00016865919],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019227382,0.000011202484,0.97570944,0.000018001654,0.000044022807,0.000255884,0.0003097747,0.0007060361,0.014192412,0.00014408666,0.00018548474,0.008231417],"study_design_scores_gemma":[0.000002892891,0.000013447658,0.99786013,0.000002122273,0.00000823232,0.0002838973,0.0000927057,0.0003922422,0.0010141347,0.00009597881,0.00022953832,0.0000046247756],"about_ca_topic_score_codex":0.0013891661,"about_ca_topic_score_gemma":0.002399623,"teacher_disagreement_score":0.0013891661,"about_ca_system_score_codex":0.00017470718,"about_ca_system_score_gemma":0.00007306989,"threshold_uncertainty_score":0.003009081},"labels":[],"label_agreement":null},{"id":"W2124489922","doi":"10.1086/323618","title":"The Far-Infrared Spectrum of Hydrogenated Amorphous Carbon and the 21, 27, and 33 Micron Features in Carbon-rich Proto–Planetary Nebulae","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Planetary nebula; Physics; Astrophysics; Spectral line; Amorphous carbon; Carbon fibers; Infrared; Stars; Astronomy; Carbon star; Nebula; Infrared spectroscopy; Wavelength; Emission spectrum; Amorphous solid; Chemistry; Materials science; Optics; Raman spectroscopy; Crystallography","score_opus":0.004342828693111855,"score_gpt":0.1917232587473681,"score_spread":0.18738043005425623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124489922","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980737,0.0003616264,0.0002619037,0.000018412478,0.0000020921702,0.0000019364606,0.000078485806,0.00002247854,0.0011793841],"genre_scores_gemma":[0.9989674,0.00013320254,0.00042159128,0.00001634849,0.0000069703606,0.0000035961634,0.00018024916,0.0000038248227,0.0002667965],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999695,0.0000023852579,9.5121624e-7,0.000010512033,0.000009449239,0.000007263032],"domain_scores_gemma":[0.9998821,0.000021658016,0.00004463555,0.000010196917,0.00001067717,0.00003070297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006665706,0.00014272769,0.000085118765,0.0004893316,0.00026766545,0.00017972648,0.00021335899,0.0002100763,0.0012343075],"category_scores_gemma":[0.000117700365,0.000093449045,0.00009716079,0.00024273778,0.00025281965,0.00017480332,0.00017817783,0.00021384351,0.00017126328],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002827191,0.00013864029,0.093457334,0.00007888983,0.000047861467,0.0007455663,0.00024124407,0.00028047242,0.8928962,0.00045261486,0.0003683488,0.011010096],"study_design_scores_gemma":[0.000016153146,0.0001961914,0.9218549,0.000010542635,0.000030850773,0.0021371196,0.00013287461,0.0004972177,0.07353518,0.00035305592,0.0012260876,0.000009802695],"about_ca_topic_score_codex":0.00034089506,"about_ca_topic_score_gemma":0.0006081681,"teacher_disagreement_score":0.0012343075,"about_ca_system_score_codex":0.00012042712,"about_ca_system_score_gemma":0.00004218377,"threshold_uncertainty_score":0.0041291118},"labels":[],"label_agreement":null},{"id":"W2124501990","doi":"10.1088/0004-637x/780/2/186","title":"NGC 1266 AS A LOCAL CANDIDATE FOR RAPID CESSATION OF STAR FORMATION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Goddard Space Flight Center; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; European Space Agency; California Institute of Technology; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Star formation; Stellar population; Population","score_opus":0.006629446088014949,"score_gpt":0.2095077743750299,"score_spread":0.20287832828701496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124501990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938069,0.00026096666,0.000249716,0.00008179182,0.000018992747,0.000015737913,0.00015542691,0.000035592282,0.005374903],"genre_scores_gemma":[0.99797267,0.00007517152,0.00024662865,0.00003254227,0.000017424038,0.0000027308442,0.00029391993,0.0000046299488,0.0013542823],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992394,0.000005291594,0.000004806083,0.000017037873,0.000019656456,0.000029317769],"domain_scores_gemma":[0.99978644,0.000009217732,0.00007500589,0.000018286812,0.000016511212,0.00009454797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000090239504,0.000195974,0.00016581097,0.0005250826,0.00056696084,0.00037706897,0.00022254616,0.00027172398,0.003829934],"category_scores_gemma":[0.0002015571,0.000097358614,0.00013558386,0.00038613446,0.00028143346,0.00020468366,0.0003058865,0.00026113106,0.000911227],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034527396,0.00012608974,0.9435127,0.000042717224,0.000024507219,0.0075436737,0.00035903906,0.00015128042,0.028651174,0.00047128272,0.0011762035,0.017596167],"study_design_scores_gemma":[0.000009287492,0.00025154202,0.97592205,0.000009945662,0.000017174569,0.016602116,0.000313219,0.00022659982,0.0016340818,0.00023890381,0.0047654053,0.000009813325],"about_ca_topic_score_codex":0.002898722,"about_ca_topic_score_gemma":0.0078053614,"teacher_disagreement_score":0.003829934,"about_ca_system_score_codex":0.00020971628,"about_ca_system_score_gemma":0.00011870735,"threshold_uncertainty_score":0.012812376},"labels":[],"label_agreement":null},{"id":"W2124547815","doi":"10.1086/312624","title":"Adaptive Optics Imaging of the CLASS Gravitational Lens System B1359+154 with the Canada-France-Hawaii Telescope","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Gravitational lens; Galaxy; Lens (geology); Telescope; Astrophysics; Redshift; Mass distribution; Hubble's law; Astronomy; Adaptive optics; Optics","score_opus":0.005886498087924817,"score_gpt":0.1892752953803864,"score_spread":0.18338879729246158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124547815","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99088496,0.00013133677,0.001222739,0.00006979601,0.000005590765,0.000016700384,0.00063954276,0.00010840674,0.006920922],"genre_scores_gemma":[0.99476177,0.00006584999,0.0037828453,0.000024327142,0.0000061959154,0.000006015134,0.00040620094,0.000010602009,0.0009361824],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999261,0.0000044241783,0.0000018056534,0.000017841328,0.000026286101,0.0000235619],"domain_scores_gemma":[0.99985194,0.000010296655,0.000033707638,0.000016450744,0.000036007263,0.000051537798],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010975457,0.00020094361,0.00009782355,0.0009572305,0.00039712584,0.0002448682,0.00028962275,0.00016759026,0.0017965962],"category_scores_gemma":[0.00016506671,0.00014092258,0.00018721083,0.00074850215,0.00019293262,0.00012702984,0.00027474764,0.00016830271,0.00019943113],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060474104,0.00013319805,0.33188742,0.00013379693,0.00029550688,0.0013608589,0.0007224683,0.0064708213,0.5916178,0.0027659896,0.0044760364,0.05953135],"study_design_scores_gemma":[0.000032715077,0.00009950971,0.97465986,0.000014300093,0.00007381595,0.0006138762,0.00017782445,0.0068960744,0.012647284,0.00029010017,0.004462375,0.00003242249],"about_ca_topic_score_codex":0.13853453,"about_ca_topic_score_gemma":0.2856645,"teacher_disagreement_score":0.13853453,"about_ca_system_score_codex":0.001295195,"about_ca_system_score_gemma":0.0006414653,"threshold_uncertainty_score":0.27545637},"labels":[],"label_agreement":null},{"id":"W2124922548","doi":"10.1088/0004-637x/690/2/1883","title":"OBSCURED STAR FORMATION IN INTERMEDIATE-DENSITY ENVIRONMENTS: A<i>SPITZER</i>STUDY OF THE ABELL 901/902 SUPERCLUSTER","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Waterloo; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Star formation; Supercluster (genetic); Galaxy; Astronomy; Star cluster; Stellar density; Intergalactic star; Luminosity function; Luminosity; Galaxy merger; Chemistry","score_opus":0.00833804371015792,"score_gpt":0.19059733043001514,"score_spread":0.18225928671985722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2124922548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999683,0.000024146271,0.000014723879,0.0000047907224,3.08685e-7,7.127166e-7,0.00009064101,0.0000035055386,0.00017814424],"genre_scores_gemma":[0.9993538,0.000022675573,0.000041287192,0.0000063365314,0.0000021084709,9.971839e-7,0.00049727847,0.0000026260775,0.000072837705],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999881,0.000007229228,0.00000616595,0.000036460642,0.000023887835,0.000045257584],"domain_scores_gemma":[0.99954116,0.000023294551,0.00016707536,0.000040119387,0.0000489266,0.0001794482],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013951457,0.0002552879,0.00033348092,0.0013066044,0.00042384374,0.0006428742,0.00033672433,0.0001930386,0.00073817],"category_scores_gemma":[0.00028456785,0.00013670394,0.00023910186,0.0006807259,0.00032005867,0.00029772162,0.0006364299,0.00018104796,0.00028393453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015307576,0.00007331541,0.97586286,0.00001102711,0.000047543694,0.00035103576,0.00034799337,0.00031657296,0.02060398,0.00008961546,0.00017315296,0.001969909],"study_design_scores_gemma":[0.0000017384086,0.000016398173,0.99919397,8.264298e-7,0.000003917041,0.00009217056,0.0001052085,0.00022960502,0.00026348935,0.00001002971,0.00008095253,0.0000016454637],"about_ca_topic_score_codex":0.011553367,"about_ca_topic_score_gemma":0.013563457,"teacher_disagreement_score":0.011553367,"about_ca_system_score_codex":0.00040474956,"about_ca_system_score_gemma":0.00013366272,"threshold_uncertainty_score":0.022972286},"labels":[],"label_agreement":null},{"id":"W2125317842","doi":"10.1088/0004-637x/760/1/12","title":"SEARCH FOR GRAVITATIONAL WAVES ASSOCIATED WITH GAMMA-RAY BURSTS DURING LIGO SCIENCE RUN 6 AND VIRGO SCIENCE RUNS 2 AND 3","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Govern de les Illes Balears; Fundacja na rzecz Nauki Polskiej; National Aeronautics and Space Administration; Scottish Funding Council; Scottish Universities Physics Alliance; Leverhulme Trust; Alfred P. Sloan Foundation; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"LIGO; Physics; Gravitational wave; Neutron star; Astrophysics; Gamma-ray burst; Astronomy; Population; Black hole (networking)","score_opus":0.012273459311530269,"score_gpt":0.2522713967402562,"score_spread":0.23999793742872597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2125317842","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99889743,0.00003100007,0.00014095982,0.00002321871,0.000002208557,0.0000078158755,0.00048350135,0.00002799819,0.0003857556],"genre_scores_gemma":[0.99366236,0.000031641142,0.0009434124,0.00003369821,0.000009972102,0.00001771723,0.004843598,0.000019117015,0.00043845063],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989685,0.00023120672,0.00007109356,0.00018765414,0.00031920557,0.00022239258],"domain_scores_gemma":[0.9954952,0.0010030535,0.0017380056,0.0004018588,0.00033129854,0.001030559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018670859,0.0005152765,0.000557828,0.0022369768,0.00053013215,0.0008855859,0.00049008924,0.0006498159,0.001062651],"category_scores_gemma":[0.004161412,0.00026758894,0.0006126781,0.0008289713,0.00040930306,0.00043733776,0.0011605528,0.00053119543,0.00031237153],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050752336,0.0001313625,0.9865715,0.000014745887,0.00015764582,0.00018343933,0.00018221395,0.0016898853,0.004441403,0.00020426621,0.00052184635,0.005394236],"study_design_scores_gemma":[0.000041554926,0.00030876067,0.9906398,0.0000069549505,0.00007202261,0.0003032424,0.00016680933,0.0046471325,0.0027612918,0.00017610547,0.0008497306,0.000026604792],"about_ca_topic_score_codex":0.0038622243,"about_ca_topic_score_gemma":0.008461175,"teacher_disagreement_score":0.0038622243,"about_ca_system_score_codex":0.0004616954,"about_ca_system_score_gemma":0.00039759307,"threshold_uncertainty_score":0.009874225},"labels":[],"label_agreement":null},{"id":"W2125502568","doi":"10.1088/0004-637x/766/1/60","title":"THE<i>GALEX</i>TIME DOMAIN SURVEY. I. SELECTION AND CLASSIFICATION OF OVER A THOUSAND ULTRAVIOLET VARIABLE SOURCES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Max-Planck-Gesellschaft; Smithsonian Institution; Durham University; National Aeronautics and Space Administration; Queen's University Belfast; Queen's University; Johns Hopkins University","keywords":"Astrophysics; Physics; RR Lyrae variable; Stars; Light curve; Quasar; Flare; Amplitude; Galaxy; Blazar; Variable star; Luminosity function; Ultraviolet; Active galactic nucleus; Absolute magnitude; Astronomy; Luminosity; Gamma ray; Optics","score_opus":0.005499765650409446,"score_gpt":0.1982916389757275,"score_spread":0.19279187332531805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2125502568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.55917144,0.0013441637,0.004404282,0.000940213,0.00017511181,0.00045184355,0.3631161,0.0012365428,0.06916025],"genre_scores_gemma":[0.4153158,0.0014459346,0.01365696,0.0011111228,0.00027226406,0.0005635879,0.54253566,0.0003585608,0.024740076],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997775,0.000029172474,0.000019450652,0.00005583864,0.00006495855,0.00005311712],"domain_scores_gemma":[0.99912614,0.00007063437,0.00031142856,0.00015194457,0.00014914927,0.00019066516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000350774,0.00043952838,0.00018105295,0.0033932035,0.0002576274,0.00079396134,0.0004235558,0.00019024254,0.0044280165],"category_scores_gemma":[0.0007496272,0.00010675351,0.00016903722,0.0025698096,0.00021614016,0.00034691757,0.0010535291,0.00023708558,0.0030961183],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034151165,0.00011052031,0.6987129,0.00022333596,0.00012251487,0.00043933804,0.0004955676,0.0007324441,0.007462082,0.003526965,0.20351821,0.08431464],"study_design_scores_gemma":[0.000027538284,0.00003513454,0.8177352,0.00004847739,0.000015899392,0.00039393408,0.00020745055,0.00057404384,0.0014249051,0.00036493767,0.17915922,0.000013246157],"about_ca_topic_score_codex":0.007499269,"about_ca_topic_score_gemma":0.008172779,"teacher_disagreement_score":0.007499269,"about_ca_system_score_codex":0.0004029605,"about_ca_system_score_gemma":0.0002750084,"threshold_uncertainty_score":0.014911234},"labels":[],"label_agreement":null},{"id":"W2125552121","doi":"10.1088/0004-637x/697/2/l95","title":"SHOCKS AND BUBBLES IN A DEEP <i>CHANDRA</i> OBSERVATION OF THE COOLING FLOW CLUSTER ABELL 2052","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Cooling flow; Cluster (spacecraft); Bubble; Galaxy cluster; Classification of discontinuities; Shock wave; Redshift; Shock (circulatory)","score_opus":0.007264803371492082,"score_gpt":0.19927658125208214,"score_spread":0.19201177788059007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2125552121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981633,0.00011014277,0.00014885583,0.000051223098,0.0000066164043,0.0000072470716,0.00038749003,0.000054545948,0.0010706383],"genre_scores_gemma":[0.9985454,0.000044103974,0.00044221545,0.00006427754,0.000018825789,0.000007510904,0.0006108288,0.000013484334,0.00025345932],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998988,0.000005694553,0.0000032690405,0.00002296972,0.000020391306,0.0000489774],"domain_scores_gemma":[0.99976104,0.000022393708,0.000059742586,0.000021999205,0.000018832912,0.00011606999],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001271697,0.0003259348,0.00035001454,0.00086918235,0.00068997045,0.0005843179,0.000292709,0.0003422685,0.00092103955],"category_scores_gemma":[0.0002694306,0.00029539753,0.0002317317,0.000635438,0.00026180712,0.00020927942,0.00070076156,0.0005381995,0.00018304586],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0029266728,0.00047841456,0.41226876,0.00022273108,0.00030875247,0.0053954897,0.0018317036,0.002434163,0.54579407,0.0016228606,0.005556572,0.021159818],"study_design_scores_gemma":[0.00004326484,0.00010620888,0.99208343,0.000010727627,0.000032340206,0.0005854807,0.00013697475,0.0011591369,0.0040320153,0.00012173831,0.0016591515,0.000029621651],"about_ca_topic_score_codex":0.014732198,"about_ca_topic_score_gemma":0.025115862,"teacher_disagreement_score":0.014732198,"about_ca_system_score_codex":0.0006301467,"about_ca_system_score_gemma":0.00022239536,"threshold_uncertainty_score":0.029292941},"labels":[],"label_agreement":null},{"id":"W2125686340","doi":"10.1088/0004-637x/777/1/45","title":"[Fe II] 1.64 μm FEATURES OF JETS AND OUTFLOWS FROM YOUNG STELLAR OBJECTS IN THE CARINA NEBULA","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Outflow; Nebula; Young stellar object; Astronomy; Accretion (finance); Radiative transfer; Star formation; Stars; Optics","score_opus":0.0071548957740773,"score_gpt":0.2158399347848734,"score_spread":0.2086850390107961,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2125686340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992643,0.00016038309,0.00009286749,0.000011813073,0.0000015263847,0.000002313036,0.00009385588,0.00001732408,0.00035554692],"genre_scores_gemma":[0.9990914,0.00008220118,0.00034714362,0.0000118394255,0.00000920214,0.0000035786165,0.0002729836,0.0000036078297,0.00017804459],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999454,0.0000019062632,0.0000028834131,0.00001927317,0.000009661426,0.000020866053],"domain_scores_gemma":[0.99981874,0.00001647601,0.00008325372,0.000014044563,0.000017628518,0.000049783946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010002918,0.000270882,0.00018309648,0.0015194352,0.00034952257,0.00036825667,0.00036180814,0.00031909617,0.000467212],"category_scores_gemma":[0.00017180794,0.00016167616,0.00015139954,0.0005244676,0.00020193295,0.00019235548,0.00025539816,0.00014694237,0.00014753317],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034949897,0.00016159829,0.7929695,0.00012313252,0.00008492598,0.003203672,0.0007981661,0.0007537495,0.17097291,0.00012703109,0.0005561618,0.02989973],"study_design_scores_gemma":[0.000003672124,0.000030262107,0.99622846,0.000004850829,0.00001895377,0.00042822203,0.000060480106,0.00047477512,0.0023725573,0.000030135074,0.00034277485,0.000004952068],"about_ca_topic_score_codex":0.002839304,"about_ca_topic_score_gemma":0.0047429954,"teacher_disagreement_score":0.002839304,"about_ca_system_score_codex":0.00018594241,"about_ca_system_score_gemma":0.000075566546,"threshold_uncertainty_score":0.005645573},"labels":[],"label_agreement":null},{"id":"W2125698779","doi":"10.1088/0004-637x/699/2/l102","title":"DISCOVERY OF PULSATIONS FROM THE PULSAR J0205+6449 IN SNR 3C 58 WITH THE <i>FERMI GAMMA-RAY SPACE TELESCOPE</i>","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Astrophysics; Pulsar; Fermi Gamma-ray Space Telescope; Spitzer Space Telescope; Telescope; Luminosity; Astronomy; Flux (metallurgy); Radio telescope; Supernova remnant; Light curve; Photon; Amplitude; Crab Pulsar; Spectral index; Supernova; Galaxy; Spectral line; Optics","score_opus":0.005783515032969262,"score_gpt":0.20656619627816253,"score_spread":0.20078268124519327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2125698779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999491,0.000052686544,0.00008991784,0.000013858113,0.000003153012,0.0000021669755,0.000046840407,0.000006616422,0.00029379554],"genre_scores_gemma":[0.99917907,0.0000616247,0.00037390125,0.00002588527,0.000008458932,0.000004415893,0.00018350636,0.0000036899191,0.00015939583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999242,0.0000061277947,0.000007948012,0.000020408712,0.000023393302,0.000017943761],"domain_scores_gemma":[0.9998196,0.000015733214,0.00007753152,0.000029627412,0.000021924527,0.00003566877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017082131,0.00020331935,0.00023393879,0.0005237178,0.0003645944,0.00042322156,0.00023815947,0.00029179401,0.000706307],"category_scores_gemma":[0.00048135093,0.00013439976,0.00017877022,0.00028891285,0.0003634551,0.00013167798,0.0005522378,0.0002360073,0.0003482774],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004581835,0.00008620037,0.7817477,0.000042347834,0.000086413966,0.0041816845,0.0006426136,0.0002663078,0.19219498,0.00032708768,0.00036925502,0.019597145],"study_design_scores_gemma":[0.000024465931,0.00025181336,0.9821146,0.000019378229,0.00005503638,0.0033313914,0.00019205737,0.000489538,0.011289782,0.0001462081,0.0020742663,0.000011540082],"about_ca_topic_score_codex":0.001929054,"about_ca_topic_score_gemma":0.0028651159,"teacher_disagreement_score":0.001929054,"about_ca_system_score_codex":0.00024682566,"about_ca_system_score_gemma":0.00012188427,"threshold_uncertainty_score":0.0038356185},"labels":[],"label_agreement":null},{"id":"W2125884793","doi":"10.1086/308633","title":"Shape of the Galactic Orbits in the CNOC1 Clusters","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Elliptical galaxy; Disc; Bulge; Lenticular galaxy; Peculiar galaxy; Astronomy; Galaxy group; Galaxy cluster; Luminous infrared galaxy; Galaxy","score_opus":0.007337041810350682,"score_gpt":0.20828154472561164,"score_spread":0.20094450291526095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2125884793","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991522,0.000049270424,0.000020493575,0.000005311278,6.5133656e-7,0.0000014851188,0.00029055818,0.00000442137,0.00047564518],"genre_scores_gemma":[0.9986382,0.000036222602,0.000057359703,0.0000026760415,0.0000014202619,0.0000021232574,0.0010218741,0.000006339934,0.00023370962],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998247,0.00000914485,0.000007863666,0.000060094284,0.00003851448,0.000059700196],"domain_scores_gemma":[0.9993073,0.00005464931,0.00021967015,0.00005480265,0.00017437518,0.00018923338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014980126,0.00020599092,0.00025970562,0.002138193,0.0006311478,0.0007298806,0.00027102072,0.00017749415,0.0011823379],"category_scores_gemma":[0.001028496,0.00012537086,0.0001388257,0.0014779655,0.00032746064,0.00014700601,0.0005051447,0.0001388527,0.0002182945],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037420916,0.000017452976,0.9822035,0.00002213428,0.00003718961,0.00010601277,0.00049553294,0.0008469601,0.007866114,0.00032890076,0.00037480952,0.0073272362],"study_design_scores_gemma":[0.000002091153,0.000007619749,0.9990355,0.0000019316778,0.0000048886013,0.000037508835,0.000080234175,0.00036692657,0.00017950354,0.000019091778,0.00026189344,0.0000028344502],"about_ca_topic_score_codex":0.06762645,"about_ca_topic_score_gemma":0.06883228,"teacher_disagreement_score":0.06762645,"about_ca_system_score_codex":0.0012781043,"about_ca_system_score_gemma":0.00041970194,"threshold_uncertainty_score":0.13446563},"labels":[],"label_agreement":null},{"id":"W2126082061","doi":"10.1088/0004-637x/796/1/63","title":"A FAR-INFRARED SPECTROSCOPIC SURVEY OF INTERMEDIATE REDSHIFT (ULTRA) LUMINOUS INFRARED GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Redshift; Luminous infrared galaxy; Galaxy; Photometry (optics); Star formation; Astronomy; Population; Infrared; Far infrared; Stars","score_opus":0.008742157523702547,"score_gpt":0.2189856216554153,"score_spread":0.21024346413171274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126082061","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939313,0.00014508828,0.00024092518,0.000031847878,0.000001594424,0.000014984406,0.0033245853,0.000055559893,0.002254178],"genre_scores_gemma":[0.9879605,0.00019067984,0.0013475713,0.00007239772,0.000015673555,0.000018923321,0.009013884,0.000023655755,0.0013567824],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997962,0.000018301122,0.000011896917,0.00007112465,0.000039947372,0.00006255364],"domain_scores_gemma":[0.9993992,0.000048287602,0.00023017798,0.000065539185,0.00007471295,0.00018216827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002890597,0.00017385319,0.00017259263,0.0023253872,0.00022076459,0.0003628411,0.00032452648,0.0001744871,0.0023083813],"category_scores_gemma":[0.00027869735,0.00012834577,0.00018295704,0.0013307584,0.00016846342,0.0003035751,0.0004774664,0.00016512054,0.0009224666],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005812965,0.00009411603,0.976982,0.000030024687,0.000050163395,0.00009093523,0.00030097264,0.00017265545,0.0081358645,0.0002046476,0.0014876749,0.012392753],"study_design_scores_gemma":[0.0000018447201,0.000014915647,0.99906045,0.0000026691525,0.000005629168,0.00004908225,0.000042974825,0.000055092583,0.00014965351,0.000008209714,0.0006078125,0.0000017075474],"about_ca_topic_score_codex":0.009904023,"about_ca_topic_score_gemma":0.025838718,"teacher_disagreement_score":0.009904023,"about_ca_system_score_codex":0.00030763983,"about_ca_system_score_gemma":0.00017845532,"threshold_uncertainty_score":0.019692779},"labels":[],"label_agreement":null},{"id":"W2126113369","doi":"10.1088/0004-637x/707/1/612","title":"MULTIWAVELENGTH OBSERVATIONS OF A TeV-FLARE FROM W COMAE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Science Foundation; Science Foundation Ireland; Russian Foundation for Basic Research; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution","keywords":"Physics; Flare; Astrophysics; Gamma ray; BL Lac object; Spectral energy distribution; High energy; Astronomy; Flux (metallurgy); Blazar; Galaxy","score_opus":0.015985670942278294,"score_gpt":0.22722689808495275,"score_spread":0.21124122714267446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126113369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99779177,0.000071438415,0.00021512173,0.000033156048,0.0000052534883,0.000010014957,0.00043693295,0.000050121464,0.0013862109],"genre_scores_gemma":[0.9964837,0.000078406665,0.0009388257,0.00006175634,0.000017251179,0.000008074422,0.0016384711,0.000016243335,0.00075723423],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999851,0.000006689543,0.000004799888,0.000030255238,0.000045135195,0.00006213676],"domain_scores_gemma":[0.99968517,0.000020774141,0.00009643454,0.00004177111,0.000049842085,0.00010611847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018511045,0.0002885605,0.00031792288,0.000911421,0.00058203837,0.00048735001,0.00033961004,0.00034630988,0.0007821547],"category_scores_gemma":[0.00031786226,0.00020269473,0.00026438225,0.0009835393,0.00021813951,0.00022633746,0.00078968384,0.0003808939,0.00022194734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010234652,0.00043906897,0.7016454,0.00009968225,0.000485567,0.0031904178,0.0010974505,0.0012854532,0.24345133,0.0003326012,0.0024400598,0.044509593],"study_design_scores_gemma":[0.000019313105,0.0001152089,0.9949244,0.0000042414263,0.000024523031,0.0003539018,0.0001001382,0.0004530792,0.0022754036,0.000034335033,0.001687213,0.0000082779],"about_ca_topic_score_codex":0.011251599,"about_ca_topic_score_gemma":0.033952113,"teacher_disagreement_score":0.011251599,"about_ca_system_score_codex":0.00052846986,"about_ca_system_score_gemma":0.00017948587,"threshold_uncertainty_score":0.022372186},"labels":[],"label_agreement":null},{"id":"W2126369591","doi":"10.1088/0004-637x/797/1/26","title":"THE INFRARED MEDIUM-DEEP SURVEY. II. HOW TO TRIGGER RADIO AGNs? HINTS FROM THEIR ENVIRONMENTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Active galactic nucleus; Supermassive black hole; Galaxy; Accretion (finance); Radio galaxy; Broadband; Infrared; Spectral energy distribution; Star formation","score_opus":0.007503326818922382,"score_gpt":0.190821333785096,"score_spread":0.18331800696617362,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126369591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97165304,0.0021505984,0.0024372004,0.00029797264,0.00003852941,0.000045448036,0.011862758,0.000104409286,0.011410044],"genre_scores_gemma":[0.9824265,0.0009069099,0.0025489102,0.00024889034,0.00006219826,0.000046335113,0.010475732,0.000023510062,0.0032610593],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999846,0.000029029652,0.000008473592,0.00004529244,0.000024453275,0.00004676722],"domain_scores_gemma":[0.99954,0.000051779534,0.00016180851,0.000057734615,0.000050843057,0.0001378744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032713925,0.00021763134,0.00016834347,0.0011348699,0.00016561692,0.00048523882,0.0002621196,0.00024877102,0.0016856806],"category_scores_gemma":[0.00044711487,0.00013762314,0.00023986245,0.00071213103,0.00012849357,0.00035931333,0.00043057412,0.00022444248,0.0010158495],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000089347515,0.00003494094,0.969493,0.0000622383,0.00004819013,0.00007389832,0.00008178745,0.00018752231,0.006690269,0.00033080945,0.0016796573,0.021228313],"study_design_scores_gemma":[0.000004889392,0.00002045279,0.99602985,0.000009814254,0.000020175408,0.00007455209,0.00009358894,0.000116192736,0.0002872692,0.00010097369,0.003239373,0.0000029783262],"about_ca_topic_score_codex":0.002153459,"about_ca_topic_score_gemma":0.005458581,"teacher_disagreement_score":0.002153459,"about_ca_system_score_codex":0.0001831541,"about_ca_system_score_gemma":0.0000871983,"threshold_uncertainty_score":0.005639136},"labels":[],"label_agreement":null},{"id":"W2126409956","doi":"10.1088/0004-637x/700/1/161","title":"MID-IR LUMINOSITIES AND UV/OPTICAL STAR FORMATION RATES AT<i>z</i>&lt; 1.4","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Photometry (optics); Star formation; Spectral energy distribution; Galaxy; Stellar population; Redshift; Luminosity; Stars; Infrared; Ultraviolet; Spectroscopy; Astronomy; Luminous infrared galaxy; Optics","score_opus":0.006545062155371654,"score_gpt":0.20660911174904587,"score_spread":0.20006404959367421,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126409956","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99802774,0.00005651378,0.00007085361,0.000009310409,6.846122e-7,0.0000034806721,0.0011075166,0.000013884699,0.00070999045],"genre_scores_gemma":[0.9972909,0.000040460687,0.00014630271,0.000005272679,0.0000035793764,0.000004820971,0.0022339374,0.0000039050906,0.0002708824],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998379,0.000014648309,0.000012551966,0.00004464111,0.000025237629,0.00006501297],"domain_scores_gemma":[0.99901164,0.00013634152,0.00048655507,0.0000787079,0.00007788059,0.00020875385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002531349,0.0002147546,0.00017587835,0.002086439,0.00019483914,0.000796572,0.0003135241,0.00027034563,0.0030541136],"category_scores_gemma":[0.0007740776,0.00013616002,0.00035545084,0.001023449,0.0003140907,0.00044686516,0.00044231565,0.00023661519,0.0007627659],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023422375,0.000013672005,0.99747,0.0000042314246,0.00001948463,0.000022719765,0.000066453096,0.00013341436,0.0008692204,0.000064631604,0.000060945382,0.0012517723],"study_design_scores_gemma":[5.728818e-7,0.0000074777217,0.999608,7.045572e-7,0.0000041566473,0.00003198011,0.000033220233,0.00012701651,0.00008317721,0.000013873845,0.000089019115,7.571053e-7],"about_ca_topic_score_codex":0.004398515,"about_ca_topic_score_gemma":0.005697146,"teacher_disagreement_score":0.004398515,"about_ca_system_score_codex":0.000272328,"about_ca_system_score_gemma":0.00007980866,"threshold_uncertainty_score":0.010217011},"labels":[],"label_agreement":null},{"id":"W2126724907","doi":"10.1088/0004-637x/790/1/71","title":"OBLIQUE SHOCK BREAKOUT IN SUPERNOVAE AND GAMMA-RAY BURSTS. II. NUMERICAL SOLUTIONS FOR NON-RELATIVISTIC PATTERN SPEEDS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Shock (circulatory); Shock wave; Astrophysics; Supernova; Mechanics; Oblique shock; RADIUS; Breakout; Adiabatic process","score_opus":0.012187507437938255,"score_gpt":0.23490469432162417,"score_spread":0.2227171868836859,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126724907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.972937,0.00032292685,0.018769832,0.00027211016,0.000061873594,0.000065052816,0.0001431078,0.00013587918,0.007292299],"genre_scores_gemma":[0.9906193,0.00015896477,0.0075544636,0.00006122878,0.000012298948,0.00004641362,0.000105904575,0.000044620563,0.0013968577],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999095,0.00003312969,0.000006121157,0.00000991403,0.000019901612,0.00002143492],"domain_scores_gemma":[0.9994497,0.00027841656,0.00013130976,0.00003787604,0.000044861794,0.000057792582],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037980598,0.0003673874,0.00034157775,0.0003840385,0.00040458926,0.0007687151,0.00059870846,0.00089958264,0.0012153086],"category_scores_gemma":[0.0029415844,0.00030596615,0.00045383567,0.00025719052,0.000795623,0.00047206116,0.000772079,0.0005291881,0.00010522127],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000076258315,0.00007090231,0.0068252026,0.000039137307,0.000031319014,0.00014557285,0.000085775435,0.98356485,0.001963218,0.0049592103,0.00017810769,0.0020605118],"study_design_scores_gemma":[0.000031094885,0.00002714706,0.001111924,0.000008841435,0.00000591868,0.000020321913,0.000036208763,0.99682593,0.00037505713,0.0013411609,0.00021209531,0.000004311697],"about_ca_topic_score_codex":0.012667066,"about_ca_topic_score_gemma":0.007454918,"teacher_disagreement_score":0.012667066,"about_ca_system_score_codex":0.0007010441,"about_ca_system_score_gemma":0.00048698968,"threshold_uncertainty_score":0.025186658},"labels":[],"label_agreement":null},{"id":"W2126752041","doi":"10.1088/0004-637x/778/1/61","title":"MERGERS IN GALAXY GROUPS. I. STRUCTURE AND PROPERTIES OF ELLIPTICAL REMNANTS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Division of Materials Research; Princeton Center for Complex Materials; National Science Foundation","keywords":"Astrophysics; Physics; Bulge; Elliptical galaxy; Galaxy; Astronomy; Fundamental plane (elliptical galaxies); Luminosity; Spiral galaxy; Velocity dispersion; Galaxy merger; Lenticular galaxy","score_opus":0.007283955789196232,"score_gpt":0.1901870451152506,"score_spread":0.18290308932605437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126752041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99849725,0.00006625575,0.00055827183,0.00004456561,0.0000037912607,0.000011987238,0.00008778013,0.00002881667,0.0007012389],"genre_scores_gemma":[0.9988219,0.000035550052,0.00060097914,0.00002264784,0.0000035959722,0.000011978381,0.00023847302,0.000013609966,0.000251241],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998142,0.00004159526,0.000011414777,0.000041384126,0.000030390878,0.00006094745],"domain_scores_gemma":[0.9993286,0.00016138305,0.0001482808,0.00008909852,0.000056136632,0.00021650766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005932197,0.00045823335,0.0004212764,0.0005554299,0.0007157261,0.00086625956,0.0010869659,0.00077474694,0.0012933415],"category_scores_gemma":[0.0021574444,0.00036806488,0.00090827286,0.00043241645,0.0011437066,0.00092147,0.001133854,0.0005950295,0.00023699403],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004959803,0.00026110865,0.15841682,0.000045791374,0.0002533488,0.00042570036,0.0006899961,0.8260871,0.0060137725,0.0032966377,0.00060432195,0.0034095107],"study_design_scores_gemma":[0.00024015807,0.0004554914,0.057693858,0.000020619285,0.000098628,0.00026618133,0.00040945425,0.934463,0.0018919283,0.0027292161,0.0016895394,0.000041977866],"about_ca_topic_score_codex":0.0140148895,"about_ca_topic_score_gemma":0.007848723,"teacher_disagreement_score":0.0140148895,"about_ca_system_score_codex":0.0009084568,"about_ca_system_score_gemma":0.00031622793,"threshold_uncertainty_score":0.027866662},"labels":[],"label_agreement":null},{"id":"W2126884143","doi":"10.1088/0004-637x/789/1/11","title":"EARLY-TYPE GALAXY CORE PHASE DENSITIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Globular cluster; Galaxy; Galaxy cluster; Core (optical fiber); Luminosity; Galaxy rotation curve; Density contrast; Cluster (spacecraft); Galaxy formation and evolution","score_opus":0.011639504342350327,"score_gpt":0.23444080513225637,"score_spread":0.22280130078990604,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126884143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9856485,0.00014869962,0.0019322651,0.000023341421,0.0000026914265,0.000011522753,0.001678942,0.0001259153,0.010428093],"genre_scores_gemma":[0.9975311,0.00005203033,0.00038686203,0.0000092448745,0.0000020797586,0.0000049185996,0.0009464887,0.000008505957,0.0010587602],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993575,0.00000750109,0.0000032289056,0.000019807156,0.000014518752,0.00001915918],"domain_scores_gemma":[0.999361,0.00018889086,0.00014939618,0.00010104025,0.00011812882,0.00008150526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013334941,0.00015578348,0.000112737165,0.0007977818,0.00014461105,0.0006560173,0.00019337148,0.00013891693,0.006453848],"category_scores_gemma":[0.0010535718,0.00012208155,0.00011899476,0.0006175231,0.0002442414,0.0003396178,0.0003327762,0.00018587877,0.00148434],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015596935,0.000035204444,0.949319,0.00003984981,0.000034415116,0.00007008348,0.0003870246,0.0014322145,0.016813789,0.004567331,0.0010179079,0.026127273],"study_design_scores_gemma":[0.0000049680775,0.000041786625,0.99209505,0.000004124007,0.000008978764,0.00026054945,0.00009904698,0.0016466619,0.0022004826,0.0017924267,0.0018390752,0.0000068849795],"about_ca_topic_score_codex":0.0013461731,"about_ca_topic_score_gemma":0.002508991,"teacher_disagreement_score":0.006453848,"about_ca_system_score_codex":0.0002691302,"about_ca_system_score_gemma":0.000076218894,"threshold_uncertainty_score":0.021590233},"labels":[],"label_agreement":null},{"id":"W2126938779","doi":"10.1088/0004-637x/786/1/58","title":"UNVEILING THE INTRINSIC X-RAY PROPERTIES OF BROAD ABSORPTION LINE QUASARS WITH A RELATIVELY UNBIASED SAMPLE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Quasar; Spectral line; Gravitational lens; Kinetic energy; Line (geometry); Emission spectrum; Spectral index; Photon; Redshift","score_opus":0.013497621930447564,"score_gpt":0.20495921772490897,"score_spread":0.1914615957944614,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2126938779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99641126,0.00023180644,0.0020774773,0.000024935209,0.000004254511,0.000011142445,0.00049438974,0.00002937954,0.00071527803],"genre_scores_gemma":[0.9962682,0.00022990326,0.0018543816,0.00008001422,0.000027707107,0.000024304805,0.0011642872,0.000017018376,0.00033430746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99938786,0.00012422346,0.000053433814,0.00020412604,0.00015116445,0.000079155005],"domain_scores_gemma":[0.99749964,0.00051169546,0.0007473652,0.0006286892,0.00045141098,0.00016120955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001164646,0.00018904837,0.00027631142,0.00081074185,0.0003157194,0.00088868564,0.00034731516,0.00024810777,0.000868472],"category_scores_gemma":[0.0031814084,0.0002101402,0.00013798857,0.00065587007,0.00039262633,0.0004580185,0.00061600236,0.00022235063,0.00033179825],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040223575,0.000025714917,0.979126,0.000019438778,0.00007861294,0.00006936344,0.00020161872,0.00022476025,0.01239893,0.00027780535,0.00017420646,0.00736337],"study_design_scores_gemma":[0.000004697127,0.000036417507,0.99546033,0.0000051565316,0.000035525718,0.0001965755,0.00010178071,0.0006510112,0.0017846979,0.00019624339,0.0015232639,0.000004376859],"about_ca_topic_score_codex":0.002210204,"about_ca_topic_score_gemma":0.0052790423,"teacher_disagreement_score":0.002210204,"about_ca_system_score_codex":0.0001458153,"about_ca_system_score_gemma":0.00015272333,"threshold_uncertainty_score":0.0061593056},"labels":[],"label_agreement":null},{"id":"W2127128586","doi":"10.1086/512096","title":"The Infrared Properties of Submillimeter Galaxies: Clues from Ultradeep 70 μm Imaging","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Luminous infrared galaxy; Infrared; Luminosity; Photometric redshift; Astronomy; Population","score_opus":0.00833210655267453,"score_gpt":0.20228473891885357,"score_spread":0.19395263236617905,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127128586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979346,0.00018626382,0.00030803305,0.000024577763,0.0000019884126,0.0000016283553,0.00031055175,0.00003496617,0.0011973893],"genre_scores_gemma":[0.9988123,0.00006873166,0.0004280275,0.000022922735,0.00000732179,0.0000019499048,0.00043875392,0.000005702205,0.00021432227],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998934,0.000008612753,0.0000054660795,0.00002315613,0.00002106864,0.000048194506],"domain_scores_gemma":[0.9995447,0.000057808495,0.00021114055,0.00004135171,0.000038696733,0.00010627966],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002518712,0.00027549913,0.00016909816,0.0014505376,0.00016986721,0.0005005331,0.00021298317,0.00022833135,0.00109942],"category_scores_gemma":[0.00050876406,0.00014611385,0.0002280981,0.0007693597,0.00015861505,0.00033942895,0.00047461624,0.00020535396,0.00036650867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041036757,0.000015986125,0.98351246,0.000011618967,0.00001931788,0.000067087494,0.00009068182,0.00018483745,0.008087744,0.000105871375,0.00022540962,0.0076378933],"study_design_scores_gemma":[8.028289e-7,0.000009551516,0.998833,0.0000021168914,0.000007845593,0.00006366946,0.00004743996,0.00028316525,0.00046922316,0.000042862437,0.00023864403,0.0000018538492],"about_ca_topic_score_codex":0.0021105332,"about_ca_topic_score_gemma":0.0049082437,"teacher_disagreement_score":0.0021105332,"about_ca_system_score_codex":0.00016905462,"about_ca_system_score_gemma":0.00006241964,"threshold_uncertainty_score":0.0041965246},"labels":[],"label_agreement":null},{"id":"W2127351488","doi":"10.1088/0004-637x/775/2/129","title":"THE OPTICAL GREEN VALLEY VERSUS MID-INFRARED CANYON IN COMPACT GROUPS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Luminous infrared galaxy; Elliptical galaxy; Galaxy group; Galaxy; Astronomy; Peculiar galaxy; Compact group; Galaxy cluster","score_opus":0.01034027366657893,"score_gpt":0.21953618841931022,"score_spread":0.20919591475273128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127351488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99550194,0.00043682772,0.00026818836,0.00003946584,0.000003613542,0.00000471829,0.00010429486,0.000011249158,0.0036297152],"genre_scores_gemma":[0.9993024,0.000054713077,0.00016037023,0.000015838588,0.000005815971,0.0000022360039,0.000089775276,0.0000037896816,0.00036503174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978083,0.00002387121,0.000011513502,0.000071231276,0.00003639251,0.00007619397],"domain_scores_gemma":[0.99882084,0.00016691626,0.00058433716,0.000090040274,0.00007926454,0.000258486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022639486,0.00016689878,0.00022736464,0.0026643353,0.00044480566,0.001172808,0.0002587854,0.00028630026,0.002992873],"category_scores_gemma":[0.0011966445,0.00011092595,0.00014094907,0.0015027283,0.0008696437,0.00085491117,0.0011014342,0.0002510077,0.00044157187],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002128186,0.00003798454,0.9766302,0.000028879262,0.000026686519,0.0001430738,0.0008580745,0.00012533483,0.004070262,0.0013064236,0.00022039363,0.016339853],"study_design_scores_gemma":[0.0000054366296,0.00004145469,0.9971578,0.0000115965495,0.000012006396,0.00021039123,0.0006817979,0.0001512427,0.00022684566,0.0008497465,0.0006486679,0.0000029862979],"about_ca_topic_score_codex":0.004393671,"about_ca_topic_score_gemma":0.0099413125,"teacher_disagreement_score":0.004393671,"about_ca_system_score_codex":0.000318376,"about_ca_system_score_gemma":0.00014762576,"threshold_uncertainty_score":0.01001215},"labels":[],"label_agreement":null},{"id":"W2127467964","doi":"10.1088/0004-637x/697/2/1634","title":"CLUSTERING OF LOW-REDSHIFT (<i>z</i>⩽ 2.2) QUASARS FROM THE SLOAN DIGITAL SKY SURVEY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":254,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Los Alamos National Laboratory; U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; New Mexico State University; University of Portsmouth; Universität Basel; University of Pittsburgh; Johns Hopkins University; Ohio State University; U.S. Department of Energy; Princeton University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Drexel University; National Aeronautics and Space Administration; Case Western Reserve University","keywords":"Redshift; Astrophysics; Quasar; Physics; Sky; Cosmology; Correlation function (quantum field theory); Redshift survey; Galaxy; Quantum mechanics","score_opus":0.009319960024508139,"score_gpt":0.2129285954154239,"score_spread":0.20360863539091575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127467964","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986003,0.00005064164,0.000099976445,0.000009317226,6.749697e-7,0.0000029824832,0.00083258474,0.000010257025,0.0003932441],"genre_scores_gemma":[0.99550015,0.00005749337,0.00020937149,0.0000067331243,0.0000029748637,0.0000042887864,0.003943681,0.0000047490153,0.00027057552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976164,0.00003127653,0.000017888393,0.000060557224,0.000057651727,0.00007092711],"domain_scores_gemma":[0.999236,0.000064501735,0.00029330378,0.00007532269,0.00011643576,0.00021457212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032965202,0.00014684013,0.00022796699,0.0023012748,0.0003077721,0.0005297289,0.00027459234,0.00013353571,0.0008300174],"category_scores_gemma":[0.0006140888,0.00009986401,0.00015714664,0.002038172,0.0002932291,0.0001959103,0.00049847434,0.00014908123,0.00033504146],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036257443,0.00001980452,0.9945457,0.000012734492,0.000031888358,0.000042829404,0.0002554612,0.00029317389,0.0013962795,0.00013184988,0.00047011385,0.0027639323],"study_design_scores_gemma":[0.0000010940846,0.0000059986955,0.99944824,9.841116e-7,0.0000026885455,0.000017018565,0.00006802825,0.00018318348,0.00005402993,0.000015534286,0.00020168026,0.000001552329],"about_ca_topic_score_codex":0.040299356,"about_ca_topic_score_gemma":0.0633772,"teacher_disagreement_score":0.040299356,"about_ca_system_score_codex":0.00048439036,"about_ca_system_score_gemma":0.00024368132,"threshold_uncertainty_score":0.080129564},"labels":[],"label_agreement":null},{"id":"W2127556270","doi":"10.1086/428929","title":"New Solar Opacities, Abundances, Helioseismology, and Neutrino Fluxes","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":633,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Helioseismology; Opacity; Physics; Neutrino; Radiative transfer; Standard solar model; Solar neutrino; Astrophysics; Convection zone; Flux (metallurgy); Radiative flux; Abundance of the chemical elements; Helium; Nuclear physics; Optics; Neutrino oscillation; Chemistry; Stars; Atomic physics","score_opus":0.012366000018641103,"score_gpt":0.2639038634945912,"score_spread":0.25153786347595014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127556270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8706881,0.0006172109,0.09966663,0.0005594631,0.00016705581,0.000048671634,0.0012666158,0.0007614871,0.026224872],"genre_scores_gemma":[0.9816871,0.0004155616,0.015136926,0.000067720925,0.000070789225,0.00004276893,0.0007660139,0.00015967408,0.0016533976],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995184,0.000092936025,0.000024346547,0.00011725907,0.00019699208,0.000050146995],"domain_scores_gemma":[0.9990582,0.0002371049,0.00019819984,0.00027014108,0.00012841354,0.00010803907],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009878074,0.00076345267,0.00064843043,0.00094236864,0.00046345475,0.0023847427,0.0017629729,0.0007233935,0.0021037823],"category_scores_gemma":[0.0034452984,0.0006566932,0.00097223633,0.00084270973,0.0010463274,0.0032139414,0.0014207824,0.001392882,0.00046670745],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002625398,0.0001609145,0.09105475,0.00011096298,0.00019942179,0.00027264605,0.0005949648,0.7642408,0.007233895,0.10838629,0.002097065,0.02538574],"study_design_scores_gemma":[0.0002306337,0.00011613148,0.032842178,0.00006441083,0.00015341495,0.0005388379,0.00020335578,0.83887005,0.009681631,0.09798548,0.019159248,0.00015459461],"about_ca_topic_score_codex":0.00495855,"about_ca_topic_score_gemma":0.003668399,"teacher_disagreement_score":0.00495855,"about_ca_system_score_codex":0.0018220318,"about_ca_system_score_gemma":0.0005133555,"threshold_uncertainty_score":0.013219774},"labels":[],"label_agreement":null},{"id":"W2127631056","doi":"10.1086/517991","title":"Deep Searches for Radio Pulsations and Bursts from Four Southern Anomalous X‐Ray Pulsars","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Luminosity; Flux (metallurgy); Epoch (astronomy); Radio frequency; Conjunction (astronomy)","score_opus":0.02059737344868929,"score_gpt":0.3077833989859983,"score_spread":0.28718602553730904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127631056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996425,0.000037947066,0.00006774854,0.0000098156515,8.3854854e-7,0.0000017746282,0.000040861123,0.0000042397874,0.00019434316],"genre_scores_gemma":[0.9983797,0.00010334109,0.00055879203,0.000016096978,0.000006994139,0.0000042905112,0.0005038038,0.0000032643977,0.00042365343],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998431,0.000015826361,0.000013497017,0.000038250753,0.00003998904,0.000049209088],"domain_scores_gemma":[0.9994355,0.00009831131,0.00017550273,0.000057713056,0.000049072918,0.00018390722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023091212,0.0002762198,0.000307468,0.0011789623,0.00047755375,0.00060740573,0.00027546604,0.00022465314,0.000885259],"category_scores_gemma":[0.0005651383,0.00022121762,0.0001552683,0.0007087161,0.0003284812,0.00033876105,0.0010685526,0.0003280806,0.00016620161],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003645092,0.00011353832,0.9009847,0.000048763814,0.000055161916,0.00063181604,0.001294225,0.00029712802,0.06726838,0.00018965591,0.00013976924,0.02861232],"study_design_scores_gemma":[0.000024091276,0.00036343106,0.99149394,0.0000063437046,0.000047742917,0.0008627797,0.0005068543,0.00047601684,0.0042753196,0.00016768638,0.0017633835,0.000012492978],"about_ca_topic_score_codex":0.0015474984,"about_ca_topic_score_gemma":0.0029203964,"teacher_disagreement_score":0.0015474984,"about_ca_system_score_codex":0.00018087661,"about_ca_system_score_gemma":0.00019489934,"threshold_uncertainty_score":0.0030770302},"labels":[],"label_agreement":null},{"id":"W2127828980","doi":"10.1088/0004-637x/768/2/104","title":"THE STRUCTURE OF THE MERGING RCS 231953+00 SUPERCLUSTER AT<i>z</i>∼ 0.9","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University","funders":"Fondo de Financiamiento de Centros de Investigación en Áreas Prioritarias; Natural Sciences and Engineering Research Council of Canada; Fonds Québécois de la Recherche sur la Nature et les Technologies; National Research Foundation","keywords":"Supercluster (genetic); Astrophysics; Physics; Redshift; Galaxy cluster; Galaxy; Cluster (spacecraft); Substructure; Astronomy; Galaxy groups and clusters; Chemistry","score_opus":0.0039038498304966125,"score_gpt":0.18624488730783573,"score_spread":0.18234103747733912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127828980","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97902554,0.00029734676,0.0003297628,0.00042432066,0.000032188113,0.000021041124,0.0015209316,0.00031257662,0.018036306],"genre_scores_gemma":[0.99623376,0.000041680523,0.00047945653,0.0000717359,0.000016032169,0.000007699643,0.0021243894,0.000048841408,0.0009764058],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987686,0.0000066735565,0.000004174536,0.000039807786,0.000032016334,0.00004044755],"domain_scores_gemma":[0.999183,0.00006061419,0.00019032827,0.00006494463,0.0001645824,0.00033642692],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013522002,0.00014586243,0.0002537102,0.0011019222,0.0011449913,0.0012427742,0.00071545126,0.000443055,0.004622584],"category_scores_gemma":[0.00074667623,0.00022581172,0.0002079634,0.0008975818,0.00073221856,0.0004368929,0.0012371547,0.0004886297,0.0008154304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014287372,0.0004228687,0.7963349,0.00019402741,0.0002955277,0.0024358097,0.0035767974,0.016980818,0.079372704,0.018755784,0.032338608,0.047863334],"study_design_scores_gemma":[0.00005716564,0.00008953103,0.96296954,0.000034266508,0.00006510037,0.00032579596,0.0012558118,0.01991738,0.0031572531,0.0015476289,0.010539771,0.000040604646],"about_ca_topic_score_codex":0.037612215,"about_ca_topic_score_gemma":0.028763859,"teacher_disagreement_score":0.037612215,"about_ca_system_score_codex":0.0013296569,"about_ca_system_score_gemma":0.0010019973,"threshold_uncertainty_score":0.074786544},"labels":[],"label_agreement":null},{"id":"W2127928502","doi":"10.1088/0004-637x/760/1/5","title":"BISPECTRUM OF THE SUNYAEV-ZEL'DOVICH EFFECT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Bispectrum; Cosmic microwave background; Physics; Astrophysics; Amplitude; Redshift; Spectral density; Sunyaev–Zel'dovich effect; Matter power spectrum; Galaxy; Optics; Statistics","score_opus":0.004745152979222776,"score_gpt":0.2072008344395303,"score_spread":0.2024556814603075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2127928502","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89304584,0.0014161603,0.080860436,0.00043272285,0.000058688245,0.000047530273,0.00039812512,0.00042521005,0.023315294],"genre_scores_gemma":[0.99646497,0.00021303802,0.002446785,0.000025954207,0.00002337823,0.000011613751,0.000089959234,0.000053225936,0.00067108404],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998586,0.000031055864,0.000005530604,0.000027809718,0.00004438868,0.000032729597],"domain_scores_gemma":[0.9988587,0.00050309533,0.00032517302,0.00012357191,0.00006355007,0.0001258697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052082544,0.00033281615,0.00032812753,0.0013041022,0.00030353747,0.00046126806,0.00048050968,0.00022324645,0.0026678245],"category_scores_gemma":[0.0028079038,0.0001547554,0.00043051972,0.0005234019,0.0005089001,0.0005117996,0.00080212107,0.0004527755,0.00016631371],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050267566,0.00009800209,0.12661639,0.00028891503,0.00036861774,0.0017037772,0.0007044109,0.09947336,0.07255314,0.62028766,0.0029785943,0.07442455],"study_design_scores_gemma":[0.00011970236,0.0002108799,0.34848306,0.000088815206,0.00016705981,0.0011978145,0.00018373285,0.43276787,0.01246264,0.19038084,0.013760676,0.00017684739],"about_ca_topic_score_codex":0.0014020136,"about_ca_topic_score_gemma":0.0009947517,"teacher_disagreement_score":0.0026678245,"about_ca_system_score_codex":0.00043819132,"about_ca_system_score_gemma":0.00023754557,"threshold_uncertainty_score":0.008924723},"labels":[],"label_agreement":null},{"id":"W2128002903","doi":"10.1088/0004-637x/701/1/471","title":"LUMINOSITY FUNCTIONS OF LMXBs IN CENTAURUS A: GLOBULAR CLUSTERS VERSUS THE FIELD","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Luminosity; Field (mathematics); Luminosity function; Centaurus A; Cosmology","score_opus":0.012673889299390957,"score_gpt":0.24295077682601757,"score_spread":0.23027688752662662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128002903","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991709,0.00013839974,0.0001693978,0.000007932193,9.964025e-7,0.0000014890567,0.0000808519,0.00002202599,0.00040802802],"genre_scores_gemma":[0.999559,0.000031093965,0.000086965745,0.000005324423,0.0000032319244,0.0000019753193,0.00015865873,0.000005916497,0.00014790255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984443,0.000022377364,0.000008576766,0.00005177432,0.000020639565,0.000052208812],"domain_scores_gemma":[0.99836046,0.000554528,0.00039102617,0.000122036414,0.00014872788,0.0004231629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050511747,0.00030092892,0.0002819577,0.0032297645,0.0003105439,0.0009062277,0.00033720362,0.00040491417,0.0011308882],"category_scores_gemma":[0.001677808,0.000118302356,0.00020907179,0.0012448451,0.0004314676,0.00036893523,0.00069809833,0.00021429847,0.00041937895],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038661968,0.00003875808,0.97487086,0.000033098564,0.00007828287,0.00020235151,0.0006118924,0.0021786385,0.011336325,0.0005115506,0.00023655753,0.009515027],"study_design_scores_gemma":[0.0000043409163,0.000036559322,0.995587,0.0000045626575,0.00001423489,0.00011988083,0.00017476926,0.0029564167,0.00077146414,0.00017369453,0.00015146338,0.0000055545524],"about_ca_topic_score_codex":0.0069649043,"about_ca_topic_score_gemma":0.0036161784,"teacher_disagreement_score":0.0069649043,"about_ca_system_score_codex":0.0006798516,"about_ca_system_score_gemma":0.000116547,"threshold_uncertainty_score":0.013848722},"labels":[],"label_agreement":null},{"id":"W2128006453","doi":"10.1088/0004-637x/733/1/29","title":"REDSHIFT DETERMINATION AND CO LINE EXCITATION MODELING FOR THE MULTIPLY LENSED GALAXY HLSW-01","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Lethbridge","funders":"Science and Technology Facilities Council","keywords":"Redshift; Galaxy; Spectral line; Millimeter; Line (geometry); Emission spectrum; Excitation; Luminosity","score_opus":0.04088260970802956,"score_gpt":0.2728474784907234,"score_spread":0.23196486878269382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128006453","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967236,0.000058485704,0.002515068,0.000021698981,0.0000012334951,0.000005650458,0.00014184939,0.00006297735,0.00046960468],"genre_scores_gemma":[0.99805546,0.000037706155,0.0013158245,0.000008947392,0.000002995855,0.000003796753,0.00039735218,0.0000115567,0.00016642577],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998454,0.00002183139,0.0000075373264,0.00005832768,0.00003016892,0.00003670782],"domain_scores_gemma":[0.9995009,0.000101927915,0.00016945068,0.00008422902,0.00004942308,0.00009404989],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040579174,0.00042981564,0.0002558483,0.00069404446,0.00021997269,0.00056086364,0.0006272963,0.00039452277,0.0005544931],"category_scores_gemma":[0.00090839533,0.00024024994,0.00038054315,0.00039104966,0.0003189523,0.00036462708,0.0005116901,0.00028788863,0.00020175493],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015963335,0.00008709361,0.7628189,0.00003125435,0.00013866289,0.0003818623,0.00025856498,0.19789591,0.018135052,0.0033825594,0.00047742462,0.016233066],"study_design_scores_gemma":[0.000028605758,0.00008627851,0.32050198,0.000007829439,0.00004567871,0.00013183257,0.00010079776,0.6722583,0.004503255,0.0011369995,0.0011677251,0.000030818992],"about_ca_topic_score_codex":0.030857177,"about_ca_topic_score_gemma":0.021720087,"teacher_disagreement_score":0.030857177,"about_ca_system_score_codex":0.0015569631,"about_ca_system_score_gemma":0.0003234448,"threshold_uncertainty_score":0.061355114},"labels":[],"label_agreement":null},{"id":"W2128026783","doi":"10.1088/0004-637x/798/2/116","title":"THE EFFECT OF MAGNETIC TOPOLOGY ON THERMALLY DRIVEN WIND: TOWARD A GENERAL FORMULATION OF THE BRAKING LAW","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Topology (electrical circuits); Physics; Angular momentum; Zeeman effect; Magnetic field; Magnetic dipole; Astrophysics; Magnetic monopole; Spin (aerodynamics); Classical mechanics; Quantum mechanics; Electrical engineering","score_opus":0.007825527057742651,"score_gpt":0.23629382696422696,"score_spread":0.22846829990648432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128026783","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.29187632,0.004395129,0.5487158,0.0056893635,0.0014868707,0.00012056,0.00029522265,0.0007900869,0.1466307],"genre_scores_gemma":[0.96437854,0.0024728568,0.01575035,0.00067128695,0.0010623906,0.0000707677,0.00010485053,0.00048753407,0.015001388],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997241,0.00010459187,0.000009652464,0.00004818313,0.000066066306,0.000047484868],"domain_scores_gemma":[0.999008,0.00032243753,0.00014687644,0.00020610748,0.00014372916,0.00017294195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00085555285,0.00078034523,0.0012286538,0.0007826869,0.0009232704,0.0027640802,0.0021224248,0.0016772522,0.008186071],"category_scores_gemma":[0.0043299063,0.000594457,0.0007238714,0.0004923109,0.0030108015,0.005528329,0.0018275593,0.0022040093,0.0007625631],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000035557314,0.00003936865,0.0003518597,0.00007997818,0.000016500857,0.0001439842,0.00014271896,0.03847698,0.004203249,0.9494585,0.0015702994,0.005480972],"study_design_scores_gemma":[0.00003408941,0.000051971914,0.0011008785,0.00002551765,0.00001397801,0.0001437341,0.00006751655,0.28007314,0.0004515194,0.7162632,0.0017317374,0.00004274698],"about_ca_topic_score_codex":0.0009411944,"about_ca_topic_score_gemma":0.0008905945,"teacher_disagreement_score":0.008186071,"about_ca_system_score_codex":0.00045531397,"about_ca_system_score_gemma":0.0004316961,"threshold_uncertainty_score":0.027385116},"labels":[],"label_agreement":null},{"id":"W2128270775","doi":"10.1086/591307","title":"Fundamental Plane of Sunyaev‐Zel’dovich Clusters","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Intracluster medium; Galaxy cluster; Cluster (spacecraft); Fundamental plane (elliptical galaxies); Redshift; Astrophysics; Virial theorem; Statistical physics; Galaxy","score_opus":0.009423208864385088,"score_gpt":0.20746161886426548,"score_spread":0.1980384099998804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128270775","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9814043,0.00026164387,0.0012833285,0.00033086145,0.000033401455,0.000010396735,0.00032406833,0.000030974043,0.01632106],"genre_scores_gemma":[0.99764806,0.00008337337,0.0002985527,0.000028999779,0.000032534197,0.000009409124,0.0003554717,0.000010951476,0.0015326567],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99987817,0.000013684128,0.0000024021833,0.000037398997,0.000023028597,0.000045403573],"domain_scores_gemma":[0.9995009,0.00006562479,0.00011018902,0.000028964223,0.000082328566,0.00021197603],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023753697,0.00018785098,0.00030151993,0.00094529387,0.0015660968,0.0014060122,0.00046747996,0.00028999327,0.0037624154],"category_scores_gemma":[0.001011951,0.00017128632,0.00012987148,0.00040832505,0.0012304924,0.0003668794,0.0007715725,0.00059832993,0.00039545246],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009655727,0.00007121789,0.13269006,0.0000767573,0.000049683684,0.00021271226,0.0020889933,0.01806338,0.008569023,0.8011078,0.013901993,0.022202816],"study_design_scores_gemma":[0.00032476522,0.0001517092,0.539778,0.00006264137,0.000029529165,0.0002546417,0.0019824302,0.05883822,0.0017517181,0.37806147,0.01865991,0.000104979415],"about_ca_topic_score_codex":0.026360964,"about_ca_topic_score_gemma":0.011329985,"teacher_disagreement_score":0.026360964,"about_ca_system_score_codex":0.0013094054,"about_ca_system_score_gemma":0.00085378403,"threshold_uncertainty_score":0.052415013},"labels":[],"label_agreement":null},{"id":"W2128347452","doi":"10.1086/431969","title":"New Low Accretion Rate Magnetic Binary Systems and their Significance for the Evolution of Cataclysmic Variables","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"White dwarf; Accretion (finance); Binary star; Intermediate polar; Sky; Cataclysmic variable star; Stars; Magnetic field; Dynamo; Gravitational wave","score_opus":0.009238915515883624,"score_gpt":0.21046424197590372,"score_spread":0.2012253264600201,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128347452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963469,0.0015990117,0.00020116357,0.00020341565,0.000018600604,0.000004476167,0.00008991316,0.000008199691,0.0015283043],"genre_scores_gemma":[0.99921536,0.00032157637,0.00011415716,0.00003068232,0.00004517387,0.000002799854,0.00011325755,0.0000025908794,0.00015440765],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997764,0.000041241005,0.000024677522,0.00006737512,0.000036165668,0.000054181128],"domain_scores_gemma":[0.99834585,0.0003576966,0.000758186,0.000103503095,0.000064652704,0.0003701392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051048194,0.00022008846,0.00036796753,0.0014030534,0.00093364244,0.0032714133,0.00048051108,0.000611683,0.0024361403],"category_scores_gemma":[0.0017262897,0.00017299794,0.00014865652,0.0011054719,0.0009321345,0.00095976656,0.0009982117,0.00077872176,0.00029719103],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003138424,0.00006372156,0.97996026,0.00002848897,0.000020727866,0.0005693891,0.0003910336,0.00020565592,0.004972651,0.0014971306,0.00013596656,0.011841031],"study_design_scores_gemma":[0.000018113034,0.000052370386,0.9944593,0.000011911535,0.00001581062,0.0013621381,0.00032081854,0.0006273533,0.00041477664,0.0017482762,0.00095755246,0.000011706438],"about_ca_topic_score_codex":0.0013676976,"about_ca_topic_score_gemma":0.0015942173,"teacher_disagreement_score":0.0032714133,"about_ca_system_score_codex":0.0006319122,"about_ca_system_score_gemma":0.00024985397,"threshold_uncertainty_score":0.0081496835},"labels":[],"label_agreement":null},{"id":"W2128453291","doi":"10.1088/0004-637x/757/1/90","title":"FOUR HIGHLY DISPERSED MILLISECOND PULSARS DISCOVERED IN THE ARECIBO PALFA GALACTIC PLANE SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Millisecond pulsar; Pulsar; Galactic plane; Binary pulsar; Population; Binary number; White dwarf; Orbital plane","score_opus":0.02816316822438209,"score_gpt":0.31119173524543003,"score_spread":0.28302856702104795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128453291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965649,0.0003025829,0.00023431862,0.000079468446,0.000007802803,0.000010428775,0.0003837458,0.000020637694,0.0023960278],"genre_scores_gemma":[0.9970816,0.00033200913,0.0006766653,0.00006724,0.00002479722,0.000011941738,0.0012173355,0.000006147338,0.00058215787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998462,0.000016366334,0.0000069522766,0.000040828196,0.000050753395,0.000038839753],"domain_scores_gemma":[0.9996043,0.000049474456,0.00016003712,0.00003793577,0.00006787471,0.0000803399],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000199399,0.00022389062,0.0001649984,0.0015656555,0.00049023546,0.0004985404,0.0002588809,0.00026611178,0.0007765557],"category_scores_gemma":[0.0005933591,0.00015963586,0.00010062002,0.0012221524,0.00028912033,0.00027190562,0.00061437447,0.00026679033,0.00021782838],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013881655,0.000047568486,0.96603715,0.000033360204,0.00005931194,0.00068713253,0.0004990519,0.00010821835,0.0096821925,0.00022840606,0.0009727093,0.021505982],"study_design_scores_gemma":[0.000010360343,0.000033117925,0.99587303,0.0000056877025,0.000014299181,0.0005622954,0.00014852462,0.00010797269,0.00035441766,0.000041625277,0.0028452838,0.0000033413328],"about_ca_topic_score_codex":0.0151865585,"about_ca_topic_score_gemma":0.03308288,"teacher_disagreement_score":0.0151865585,"about_ca_system_score_codex":0.00053256017,"about_ca_system_score_gemma":0.0002693389,"threshold_uncertainty_score":0.03019631},"labels":[],"label_agreement":null},{"id":"W2128469676","doi":"10.1088/0004-637x/744/1/1","title":"TIME-DEPENDENT SEARCHES FOR POINT SOURCES OF NEUTRINOS WITH THE 40-STRING AND 22-STRING CONFIGURATIONS OF ICECUBE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Physics; Blazar; Flare; Neutrino; Fermi Gamma-ray Space Telescope; Astrophysics; Neutrino detector; Astronomy; Sky; Spitzer Space Telescope; Neutrino astronomy; Telescope; Gamma ray; Neutrino oscillation; Particle physics","score_opus":0.01824495614645672,"score_gpt":0.21782993814876717,"score_spread":0.19958498200231045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128469676","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98641497,0.00011667685,0.0025809708,0.000062237326,0.000019030069,0.000048233367,0.0021988207,0.00043870078,0.008120366],"genre_scores_gemma":[0.97514445,0.00009146343,0.01574607,0.00003747199,0.000018116176,0.000108438624,0.007135523,0.00012948163,0.0015890156],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99914014,0.00030649934,0.000035317964,0.00015972654,0.00017662808,0.0001815964],"domain_scores_gemma":[0.99891746,0.00035195236,0.00014795655,0.00027164211,0.0001587215,0.00015235969],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011705763,0.00048114706,0.0006242635,0.0011149102,0.00038819082,0.0009699326,0.0008323844,0.00043339783,0.003220391],"category_scores_gemma":[0.0019401312,0.00034101744,0.00049811194,0.0015963392,0.00044442274,0.00077900745,0.0011114802,0.00029419884,0.00040575073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.015236457,0.0011375847,0.41986388,0.00032353922,0.0012359888,0.0023825965,0.0008625236,0.3163392,0.07759428,0.016889647,0.022078097,0.12605618],"study_design_scores_gemma":[0.0013021189,0.0020204845,0.30357525,0.00008199039,0.00038970768,0.0010521476,0.0011824154,0.58694667,0.058377635,0.009989078,0.03477142,0.00031109192],"about_ca_topic_score_codex":0.0069218427,"about_ca_topic_score_gemma":0.010092359,"teacher_disagreement_score":0.0069218427,"about_ca_system_score_codex":0.00093202124,"about_ca_system_score_gemma":0.0006668418,"threshold_uncertainty_score":0.01376307},"labels":[],"label_agreement":null},{"id":"W2128619048","doi":"10.1086/342146","title":"A<i>Far Ultraviolet Spectroscopic Explorer</i>Survey of Interstellar Molecular Hydrogen in Translucent Clouds","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":323,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Extinction (optical mineralogy); Molecular cloud; Hydrogen molecule; Ultraviolet; Mean kinetic temperature; Hydrogen; Line-of-sight; Astrophysics; Far ultraviolet; Physics; Spectral line; Absorption (acoustics); Astronomy; Optics; Stars","score_opus":0.018961015098655668,"score_gpt":0.23737699906626947,"score_spread":0.2184159839676138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128619048","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.960926,0.0019454499,0.0009911206,0.001796323,0.00012820013,0.000077680896,0.010055978,0.00025448538,0.02382485],"genre_scores_gemma":[0.96736944,0.0008211746,0.0023003279,0.001588296,0.00029748204,0.000039404575,0.012327661,0.00007276795,0.015183294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998864,0.0000072855287,0.0000040455247,0.000025665,0.000033331682,0.000043262815],"domain_scores_gemma":[0.9994604,0.00005630742,0.00012404131,0.000035201654,0.00008869576,0.00023540024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041816954,0.00025566103,0.00022694057,0.0013312922,0.0008111143,0.0005757432,0.00048354108,0.00053400046,0.008119247],"category_scores_gemma":[0.0002818545,0.00010352299,0.00020762005,0.00087794836,0.0002408258,0.0005929812,0.00074320793,0.00035355234,0.0010755741],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014401178,0.0006236234,0.66844606,0.00033913154,0.00027236348,0.0018550855,0.0005786129,0.0012941731,0.19434437,0.002264663,0.039616298,0.08892557],"study_design_scores_gemma":[0.000049233262,0.00028987837,0.973651,0.000026007821,0.000060165643,0.00043155745,0.00035747205,0.0003554436,0.0064014364,0.00049818674,0.017863814,0.000015767773],"about_ca_topic_score_codex":0.007676862,"about_ca_topic_score_gemma":0.019248463,"teacher_disagreement_score":0.008119247,"about_ca_system_score_codex":0.00038250117,"about_ca_system_score_gemma":0.00046009885,"threshold_uncertainty_score":0.027161598},"labels":[],"label_agreement":null},{"id":"W2128750553","doi":"10.1086/309435","title":"Discovery of Two High Magnetic Field Radio Pulsars","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":259,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Supernova; Magnetic dipole; Magnetic field; Supernova remnant; Rotation period; Astronomy; Orbital period; Dipole; Glitch; Stars; Quantum mechanics; Optics","score_opus":0.006643558092372019,"score_gpt":0.2883293708732527,"score_spread":0.28168581278088073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2128750553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808216,0.00032341,0.00075139734,0.000060014838,0.000025582554,0.000007929719,0.00006468275,0.00002661124,0.0006582318],"genre_scores_gemma":[0.9976053,0.00015543404,0.0011632133,0.00009392301,0.00006225303,0.000010842949,0.00041685734,0.000008083811,0.0004841324],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977285,0.000018681125,0.00001707601,0.000085495514,0.0000530459,0.000052940075],"domain_scores_gemma":[0.99925023,0.00013687859,0.00020589672,0.00006071495,0.00006133024,0.00028497793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025637844,0.0003344112,0.0003606483,0.0010069823,0.00049315847,0.0010632257,0.00047563977,0.00059177633,0.0006342252],"category_scores_gemma":[0.0007896759,0.00028104894,0.00019829458,0.00042947594,0.00057007495,0.00035574066,0.0011357194,0.0006313415,0.00032562454],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005457881,0.00019876758,0.6696732,0.00012895577,0.00018873395,0.012066883,0.0015115448,0.00030656814,0.2605816,0.0014900093,0.0009122318,0.052395705],"study_design_scores_gemma":[0.00009460533,0.0007582732,0.9264812,0.000018609771,0.0001343663,0.022829922,0.00045167594,0.0006720078,0.03725433,0.00063385355,0.010608374,0.00006271706],"about_ca_topic_score_codex":0.0003039907,"about_ca_topic_score_gemma":0.00037837902,"teacher_disagreement_score":0.0010632257,"about_ca_system_score_codex":0.0002089827,"about_ca_system_score_gemma":0.00011484551,"threshold_uncertainty_score":0.002121687},"labels":[],"label_agreement":null},{"id":"W2129036998","doi":"10.1088/0004-637x/790/1/14","title":"MOA-2013-BLG-220Lb: MASSIVE PLANETARY COMPANION TO GALACTIC-DISK HOST","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Host (biology); Key (lock); Biological evolution","score_opus":0.009319418241603818,"score_gpt":0.2173067601576408,"score_spread":0.207987341916037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129036998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9135252,0.0020849295,0.0022401095,0.0039185705,0.0010732339,0.00017062502,0.010954113,0.0016128506,0.06442046],"genre_scores_gemma":[0.96364105,0.0002817704,0.002021372,0.001164658,0.00020136434,0.00003694691,0.009583086,0.00014751322,0.022922298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989736,0.0000057903253,0.0000050822227,0.000033883793,0.000020617972,0.000037165693],"domain_scores_gemma":[0.99966073,0.00001716813,0.000035644298,0.000032197055,0.00003388311,0.0002204178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011918032,0.000254328,0.00027571435,0.0009867206,0.001984895,0.001292961,0.00041273577,0.0012057435,0.011012173],"category_scores_gemma":[0.0005302166,0.000125757,0.00020302278,0.0006843696,0.00039251315,0.0006331577,0.001248588,0.0008158428,0.0040421817],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002118585,0.0009634965,0.47235775,0.00043089822,0.00019216986,0.10752721,0.0027977368,0.0005967187,0.09588798,0.019786313,0.17552105,0.121820025],"study_design_scores_gemma":[0.00013438334,0.0005335629,0.4295339,0.00014037984,0.0000749642,0.122054584,0.0025417118,0.001722303,0.011294397,0.0053118556,0.42657995,0.000077943514],"about_ca_topic_score_codex":0.0055212895,"about_ca_topic_score_gemma":0.009116837,"teacher_disagreement_score":0.011012173,"about_ca_system_score_codex":0.00084362086,"about_ca_system_score_gemma":0.00044297666,"threshold_uncertainty_score":0.036839366},"labels":[],"label_agreement":null},{"id":"W2129141017","doi":"10.1086/504035","title":"Magnetic Fields in Starburst Galaxies and the Origin of the FIR‐Radio Correlation","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":228,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Bremsstrahlung; Magnetic field; Galaxy; Spiral galaxy; Cosmic ray; Spectral line; Ionization; Electron; Synchrotron","score_opus":0.00418260154257502,"score_gpt":0.1858558816865188,"score_spread":0.18167328014394377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129141017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99916744,0.00013696557,0.0003070153,0.0000128590755,7.2953264e-7,0.0000010854167,0.00007232516,0.000008766736,0.0002928055],"genre_scores_gemma":[0.99971944,0.000026880507,0.00012992037,0.0000025843076,0.0000019451682,9.2448596e-7,0.00008428537,0.0000016556359,0.000032432676],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998092,0.00003861833,0.000013823659,0.000057787078,0.000024646579,0.00005597055],"domain_scores_gemma":[0.99604034,0.0010957592,0.0019532929,0.00033963507,0.00022121902,0.00034974318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005433236,0.00023279335,0.00028792568,0.0012499272,0.00026388766,0.00069534045,0.0002871433,0.00022056008,0.00059727044],"category_scores_gemma":[0.0031727701,0.00015861505,0.00014791997,0.0007000743,0.00046523524,0.00025550605,0.0003604696,0.00022471143,0.00017228565],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000071693714,0.000009273285,0.99361515,0.0000063680045,0.000016688746,0.00002559499,0.000089724206,0.0004011611,0.0029064408,0.00013018715,0.00003003138,0.0026976587],"study_design_scores_gemma":[0.0000028170136,0.00002002734,0.99858356,0.0000029626801,0.0000069385856,0.000066360444,0.000039171897,0.0006989029,0.00034093347,0.00014643118,0.00009011955,0.0000018096619],"about_ca_topic_score_codex":0.003078178,"about_ca_topic_score_gemma":0.0030524866,"teacher_disagreement_score":0.003078178,"about_ca_system_score_codex":0.00032170635,"about_ca_system_score_gemma":0.00009899873,"threshold_uncertainty_score":0.0061205626},"labels":[],"label_agreement":null},{"id":"W2129435656","doi":"10.1088/0004-637x/797/2/92","title":"A HARD X-RAY POWER-LAW SPECTRAL CUTOFF IN CENTAURUS X-4","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Centaurus A; Cutoff; Astrophysics; X-ray; X-ray astronomy; Astronomy; Power law; Active galactic nucleus; Galaxy; Optics; Quantum mechanics","score_opus":0.009465053369872835,"score_gpt":0.22008386578334177,"score_spread":0.21061881241346894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129435656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989876,0.00010324528,0.00015203278,0.000012971816,0.0000021339206,0.000001671839,0.000030180116,0.000021917755,0.00068824086],"genre_scores_gemma":[0.9995658,0.000031494506,0.00007236221,0.000008232209,0.00000339243,0.0000023299403,0.000091381284,0.000006232836,0.00021893506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992156,0.0000057607713,0.000005206245,0.000026975447,0.000015175455,0.000025329515],"domain_scores_gemma":[0.9997036,0.000040847375,0.00013417141,0.0000268541,0.00002251907,0.00007200064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011319131,0.00028990812,0.00028286563,0.0015396037,0.00043825046,0.0008489815,0.00039466555,0.00033899932,0.0014230893],"category_scores_gemma":[0.0006065628,0.00025687955,0.00016622095,0.0004888866,0.0005210005,0.0002635703,0.00087113486,0.0002791689,0.00032426236],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054022827,0.00008058283,0.7754737,0.000075721,0.000057627643,0.001699582,0.0007296202,0.0007455228,0.20813385,0.0009903077,0.00023154808,0.011241626],"study_design_scores_gemma":[0.0000060831885,0.00005605991,0.9947919,0.000007930986,0.0000127485455,0.0006315485,0.00011081861,0.00058691006,0.0031284336,0.00028585223,0.0003743866,0.0000074292284],"about_ca_topic_score_codex":0.0019370348,"about_ca_topic_score_gemma":0.0024478247,"teacher_disagreement_score":0.0019370348,"about_ca_system_score_codex":0.0005240591,"about_ca_system_score_gemma":0.000113747345,"threshold_uncertainty_score":0.004760742},"labels":[],"label_agreement":null},{"id":"W2129474605","doi":"10.1088/0004-637x/700/1/149","title":"A MID-INFRARED COUNTERPART TO THE MAGNETAR 1E 2259+586","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Spitzer Space Telescope; Pulsar; Astrophysics; Infrared; Flux (metallurgy); Extinction (optical mineralogy); Astronomy; Telescope; Optics; Materials science","score_opus":0.009575591225208261,"score_gpt":0.3027902522131061,"score_spread":0.2932146609878979,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129474605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99538547,0.00021195714,0.0003924756,0.00008120557,0.000031655472,0.0000047374588,0.0001604574,0.00004053201,0.003691504],"genre_scores_gemma":[0.9975182,0.00007155681,0.0009426022,0.0000803145,0.000043977372,0.0000036633817,0.00030898323,0.0000061049404,0.0010247064],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993575,0.000002602106,0.0000026596906,0.00002075299,0.000018993065,0.000019307863],"domain_scores_gemma":[0.99985373,0.000008018522,0.000055502143,0.000020966385,0.00001529846,0.000046484827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000098646946,0.00015007003,0.00021275465,0.0003416326,0.00048524878,0.00042436345,0.0003924284,0.0003818763,0.0017522916],"category_scores_gemma":[0.0001856255,0.00012585777,0.00014418864,0.00019490361,0.00027936246,0.00019468258,0.0005903806,0.00034178328,0.0006644451],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071683375,0.00024432095,0.324098,0.0002452517,0.00008452873,0.011784838,0.00076642697,0.00047266495,0.5916949,0.003921867,0.0034712811,0.06249917],"study_design_scores_gemma":[0.000051872936,0.00052409247,0.9207454,0.000026420577,0.00006712498,0.01969656,0.0003245064,0.0011080605,0.026307233,0.001272908,0.029844347,0.000031528787],"about_ca_topic_score_codex":0.00037482585,"about_ca_topic_score_gemma":0.0008653685,"teacher_disagreement_score":0.0017522916,"about_ca_system_score_codex":0.00011874109,"about_ca_system_score_gemma":0.00005804343,"threshold_uncertainty_score":0.0058619976},"labels":[],"label_agreement":null},{"id":"W2129514773","doi":"10.1088/0004-637x/693/1/691","title":"PERIOD-LUMINOSITY RELATIONS DERIVED FROM THE OGLE-III FUNDAMENTAL MODE CEPHEIDS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cepheid variable; Astrophysics; Physics; Extinction (optical mineralogy); Large Magellanic Cloud; Luminosity; Sky; Cosmic distance ladder; Astronomy; Galaxy; Stars; Optics","score_opus":0.012016273479457268,"score_gpt":0.23102989819725536,"score_spread":0.2190136247177981,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129514773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9564403,0.0018221464,0.0035731224,0.00011640125,0.000031864085,0.000022228283,0.004950652,0.000199728,0.03284363],"genre_scores_gemma":[0.99646086,0.00019803006,0.00087128155,0.0000225755,0.000017166347,0.000006707651,0.001400076,0.000036892226,0.0009864608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999938,0.0000070346186,0.0000043509567,0.00002027413,0.00001107159,0.000019204683],"domain_scores_gemma":[0.99934334,0.00029487512,0.00013511779,0.000049803853,0.000109629684,0.00006723094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026097026,0.00022259861,0.00015857058,0.0011374457,0.00030786954,0.00077025796,0.00019296222,0.0002968198,0.003975246],"category_scores_gemma":[0.0011084556,0.0001443873,0.00018208426,0.00091073394,0.0001544629,0.00036987144,0.00030354646,0.00046325426,0.0012814837],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010628838,0.00005519495,0.8476794,0.00034674694,0.00013708071,0.00048243074,0.0013396011,0.008993506,0.032060802,0.012242231,0.0062862504,0.089313835],"study_design_scores_gemma":[0.00002507003,0.000038848742,0.986893,0.000022028704,0.00003359018,0.000117270654,0.00010421042,0.00457562,0.0013157636,0.0013554877,0.005509233,0.000009757844],"about_ca_topic_score_codex":0.004938592,"about_ca_topic_score_gemma":0.010564302,"teacher_disagreement_score":0.004938592,"about_ca_system_score_codex":0.0005426089,"about_ca_system_score_gemma":0.00014049123,"threshold_uncertainty_score":0.0132985115},"labels":[],"label_agreement":null},{"id":"W2129602236","doi":"10.1086/507460","title":"Interferometric Mapping of Magnetic Fields: NGC 2071IR","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Outflow; Flattening; Magnetic field; Interferometry; Thermal emission; Bipolar outflow; Astronomy; Galaxy; Thermal; Star formation; Chemistry","score_opus":0.00973197657755655,"score_gpt":0.21660678311372963,"score_spread":0.20687480653617307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129602236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99705976,0.000054345735,0.00013508109,0.000024490966,0.000002425466,0.000003468453,0.0005078105,0.00006925002,0.0021433525],"genre_scores_gemma":[0.9982633,0.000033653472,0.00047004738,0.00001130346,0.000008827129,0.000005381886,0.0010166769,0.000010981516,0.00017991764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999199,0.000006520027,0.000002080562,0.000024056455,0.000018638917,0.000028880882],"domain_scores_gemma":[0.99974555,0.00003080265,0.00006809146,0.00002538391,0.000039752256,0.00009037729],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000800293,0.00018149319,0.00020285287,0.0013575022,0.00034562105,0.0003701044,0.00020830314,0.0002310262,0.0011310601],"category_scores_gemma":[0.00019854582,0.00013901354,0.00017482316,0.00062875554,0.00014261206,0.000092399285,0.00026373196,0.00023206271,0.0003346526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009249412,0.00024769676,0.761632,0.00011015781,0.00018124907,0.0018812174,0.0010731828,0.005447157,0.18280809,0.0009880181,0.006865698,0.037840616],"study_design_scores_gemma":[0.000009824063,0.00003407011,0.9936178,0.000007614418,0.000018958388,0.00035012947,0.00011623304,0.0021885985,0.0026042291,0.00005174482,0.0009927329,0.000008129086],"about_ca_topic_score_codex":0.008968715,"about_ca_topic_score_gemma":0.017925745,"teacher_disagreement_score":0.008968715,"about_ca_system_score_codex":0.0004188853,"about_ca_system_score_gemma":0.00017157661,"threshold_uncertainty_score":0.017832994},"labels":[],"label_agreement":null},{"id":"W2129668049","doi":"10.1086/339363","title":"Annealing of Silicate Dust by Nebular Shocks at 10 AU","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":175,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Silicate; Amorphous solid; Interplanetary dust cloud; Astrophysics; Protoplanetary disk; Pyroxene; Olivine; Chondrite; Physics; Astrobiology; Planet; Solar System; Meteorite; Mineralogy; Astronomy; Geology; Chemistry","score_opus":0.011247405315473288,"score_gpt":0.19984528157016956,"score_spread":0.18859787625469626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129668049","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982463,0.000056256777,0.0007353978,0.000009137121,0.0000030800413,0.0000037156924,0.000048992377,0.000030606614,0.00086642115],"genre_scores_gemma":[0.9996112,0.00003131011,0.00017449094,0.000004125883,0.0000014607598,0.0000018941029,0.000047528927,0.000005044461,0.0001229179],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999645,0.0000022494412,0.0000022861113,0.000009169438,0.0000073275382,0.000014520776],"domain_scores_gemma":[0.9999156,0.000030737396,0.000024537163,0.000008456324,0.000010330181,0.000010227588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006957728,0.0002113684,0.0001369743,0.00021074337,0.00021492278,0.00038877406,0.00020881578,0.00028524586,0.001181987],"category_scores_gemma":[0.0003835138,0.00015573282,0.00026922466,0.00015394138,0.0002772628,0.00023564146,0.00021143169,0.00018614392,0.00011614838],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056302,0.00016721296,0.1743371,0.00018714127,0.00024841726,0.0015816563,0.00038144173,0.37834397,0.42893463,0.004690004,0.00040855183,0.010156895],"study_design_scores_gemma":[0.000116991556,0.00043801163,0.25448453,0.000017875414,0.00010550665,0.0004519669,0.00025312856,0.6119847,0.12933868,0.0017569532,0.0010218987,0.000029685112],"about_ca_topic_score_codex":0.0046086838,"about_ca_topic_score_gemma":0.0027217786,"teacher_disagreement_score":0.0046086838,"about_ca_system_score_codex":0.00050924264,"about_ca_system_score_gemma":0.00014135838,"threshold_uncertainty_score":0.009163737},"labels":[],"label_agreement":null},{"id":"W2129709920","doi":"10.1088/0004-637x/703/2/2259","title":"ARECIBO PULSAR SURVEY USING ALFA: PROBING RADIO PULSAR INTERMITTENCY AND TRANSIENTS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"Office of Naval Research; Fonds Québécois de la Recherche sur la Nature et les Technologies; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canadian Institute for Advanced Research; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Associated Universities; Swinburne University of Technology; National Radio Astronomy Observatory; National Science Foundation","keywords":"Pulsar; Physics; Galactic plane; Duty cycle; Intermittency; Scintillation; Astrophysics; Transient (computer programming); Pulse (music); Millisecond pulsar; Rotation (mathematics); Astronomy; Detector; Stars; Optics; Meteorology; Computer science","score_opus":0.02471709675040428,"score_gpt":0.3253898379945937,"score_spread":0.3006727412441894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129709920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99270517,0.00018157213,0.0036543147,0.00005181388,0.000006932924,0.00005276955,0.0015878963,0.00034228907,0.0014171579],"genre_scores_gemma":[0.97650015,0.00023085214,0.013759554,0.00004092986,0.000040231407,0.000054826225,0.008773833,0.000059831596,0.00053972186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99944836,0.00015647177,0.000028945693,0.0000918022,0.00016914486,0.00010523146],"domain_scores_gemma":[0.99819946,0.00055942155,0.0003796081,0.0002364614,0.00040831394,0.0002167716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001262497,0.00034682796,0.00046254075,0.0020102053,0.00036549976,0.00046902816,0.00037797957,0.00023716742,0.0006454253],"category_scores_gemma":[0.0027457504,0.00012233197,0.0003037627,0.0017297553,0.00018936158,0.0002802222,0.0004022796,0.00016648174,0.00026949766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007513403,0.00018399782,0.8748566,0.00012755967,0.00019467859,0.0002441989,0.000226411,0.0048887962,0.015191957,0.00044190988,0.0028264786,0.10006606],"study_design_scores_gemma":[0.0000782379,0.0001824193,0.97075486,0.000011357257,0.000076736345,0.00035529563,0.00010206745,0.021402726,0.0032945843,0.00019242347,0.0035302627,0.000019070245],"about_ca_topic_score_codex":0.014431091,"about_ca_topic_score_gemma":0.017878411,"teacher_disagreement_score":0.014431091,"about_ca_system_score_codex":0.00032698584,"about_ca_system_score_gemma":0.00037423492,"threshold_uncertainty_score":0.028694153},"labels":[],"label_agreement":null},{"id":"W2129810220","doi":"10.1088/0004-637x/730/2/134","title":"PTF 10fqs: A LUMINOUS RED NOVA IN THE SPIRAL GALAXY MESSIER 99","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Luminosity; Spiral galaxy; Nova (rocket); Galaxy; Light curve; Spiral (railway); Universe; Red giant","score_opus":0.02804631871583363,"score_gpt":0.24046579941865678,"score_spread":0.21241948070282315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129810220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99681085,0.0003009011,0.00018573957,0.00020584922,0.0000147035325,0.0000149766265,0.00015849918,0.000039596274,0.0022688613],"genre_scores_gemma":[0.9978447,0.00021041169,0.0003352306,0.00016199132,0.000028860413,0.0000051252355,0.0003313598,0.0000052125242,0.0010769761],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998723,0.000008868227,0.000006989714,0.000039847866,0.000023717786,0.00004813015],"domain_scores_gemma":[0.99979824,0.000012023639,0.000067551526,0.000017526389,0.000009988855,0.00009466927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015826317,0.000348516,0.00019314022,0.0011175707,0.00054033677,0.00079866225,0.00027776998,0.0007501624,0.0014677437],"category_scores_gemma":[0.00033414763,0.00016650649,0.00024581977,0.00030138457,0.0005771919,0.00039947635,0.0006972087,0.00037096452,0.00038971324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007722704,0.00018644278,0.86447847,0.00006776819,0.00009110757,0.02404717,0.0014415112,0.0003089376,0.06264273,0.003497992,0.0032838192,0.039181706],"study_design_scores_gemma":[0.0000397871,0.0004330936,0.9557329,0.000032987053,0.00003843404,0.027082192,0.00058334495,0.0004372151,0.003291781,0.0008584565,0.011442998,0.000026865335],"about_ca_topic_score_codex":0.0067517464,"about_ca_topic_score_gemma":0.00639438,"teacher_disagreement_score":0.0067517464,"about_ca_system_score_codex":0.00060274755,"about_ca_system_score_gemma":0.0001490933,"threshold_uncertainty_score":0.013424873},"labels":[],"label_agreement":null},{"id":"W2129882625","doi":"10.1086/519236","title":"The Unusual Hydrocarbon Emission from the Early Carbon Star HD 100764: The Connection between Aromatics and Aliphatics","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":169,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Spectrograph; Infrared; Spectral line; Ultraviolet; Hydrocarbon; Carbon star; Carbon fibers; Wavelength; Radiation; Polycyclic aromatic hydrocarbon","score_opus":0.011366671315839927,"score_gpt":0.24075850556417766,"score_spread":0.22939183424833773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129882625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987387,0.000087456465,0.00011773628,0.000017090248,0.0000025632937,0.0000029145538,0.00015098114,0.0000091263055,0.00087345025],"genre_scores_gemma":[0.9983014,0.00007759282,0.0005797331,0.000021927131,0.000008899916,0.0000025793822,0.0005216355,0.000006434311,0.00047970764],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993193,0.0000036823321,0.0000030831773,0.000018418565,0.000023016793,0.000019903577],"domain_scores_gemma":[0.9998259,0.000030327363,0.000046150966,0.00002255054,0.00002737634,0.00004774414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000097682976,0.0002634364,0.00017391554,0.00083346857,0.0005482007,0.00043640155,0.0002598384,0.00032152113,0.0009853265],"category_scores_gemma":[0.00021513252,0.00015936288,0.00010219416,0.00090975047,0.0004350303,0.00026531654,0.00032191005,0.00028071902,0.00026405853],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048641855,0.00018042185,0.2505922,0.00010557891,0.00010275913,0.002577393,0.00030826402,0.0009981793,0.7327139,0.0003218371,0.00040933586,0.011203734],"study_design_scores_gemma":[0.000036294277,0.00015387536,0.9333236,0.000009883666,0.00004282588,0.0018263567,0.00016937625,0.0008615169,0.0612629,0.00022663664,0.0020696488,0.00001710858],"about_ca_topic_score_codex":0.0027816154,"about_ca_topic_score_gemma":0.0050818664,"teacher_disagreement_score":0.0027816154,"about_ca_system_score_codex":0.00036013348,"about_ca_system_score_gemma":0.00014845833,"threshold_uncertainty_score":0.005530894},"labels":[],"label_agreement":null},{"id":"W2129885058","doi":"10.1086/374418","title":"Geodetic Precession and Timing of the Relativistic Binary Pulsars PSR B1534+12 and PSR B1913+16","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Physics; Binary pulsar; Neutron star; Astrophysics; Precession; General relativity; Millisecond pulsar; Astronomy; X-ray pulsar; Astrometry; Theoretical physics; Stars","score_opus":0.01427760917056601,"score_gpt":0.3088454967046257,"score_spread":0.29456788753405966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2129885058","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843913,0.00013357187,0.00029870027,0.00002119831,0.0000043158416,0.000001943489,0.0000814168,0.0000145854,0.0010051941],"genre_scores_gemma":[0.99897254,0.00007647022,0.00050747243,0.000008347103,0.000006331511,0.0000030025424,0.0002103147,0.0000073544725,0.0002083348],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999074,0.000016429329,0.000008916776,0.000023446244,0.000030782172,0.000012994982],"domain_scores_gemma":[0.99950016,0.00004381818,0.0003241414,0.000043440294,0.00004578969,0.000042772364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028194615,0.00009306896,0.00013058887,0.0005687328,0.00014936978,0.0003139901,0.00015396516,0.00019230742,0.00043479545],"category_scores_gemma":[0.0010184782,0.00012202498,0.00007271143,0.00061756605,0.00026212633,0.00016534899,0.00033659983,0.00019640986,0.0001741726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011738156,0.00009429935,0.70154977,0.00009223754,0.000086381915,0.0005902012,0.000863364,0.0018997825,0.23556559,0.0034129063,0.000692196,0.05397947],"study_design_scores_gemma":[0.000011384484,0.00016617293,0.9918147,0.000005528795,0.000014293757,0.0003359344,0.00010574033,0.0010673997,0.005116017,0.00024778236,0.0011047093,0.000010444579],"about_ca_topic_score_codex":0.0025456862,"about_ca_topic_score_gemma":0.0023585304,"teacher_disagreement_score":0.0025456862,"about_ca_system_score_codex":0.00020983946,"about_ca_system_score_gemma":0.00012380295,"threshold_uncertainty_score":0.0050618052},"labels":[],"label_agreement":null},{"id":"W2130184138","doi":"10.1086/588518","title":"SiFTO: An Empirical Method for Fitting SN Ia Light Curves","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":249,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"Photometry (optics); Light curve; Physics; Supernova; Astrophysics; Luminosity distance; Redshift; Wavelength; Generalization; Filter (signal processing); Optics; Computer science; Mathematics; Mathematical analysis; Galaxy; Stars; Computer vision","score_opus":0.030422167415294268,"score_gpt":0.3249891823364386,"score_spread":0.29456701492114434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130184138","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.06095456,0.00017698342,0.81553155,0.00010931608,0.00025791686,0.00027380846,0.009684565,0.10847452,0.0045367964],"genre_scores_gemma":[0.15029305,0.00015858805,0.8026367,0.000107605476,0.0000684324,0.00050218176,0.023051195,0.015946245,0.0072360123],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99942565,0.000086179025,0.00005685601,0.00015412558,0.00018875308,0.00008857214],"domain_scores_gemma":[0.9985545,0.00033209586,0.00018384398,0.0003768731,0.00047302313,0.0000796707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015778682,0.0013007796,0.00069155206,0.0031149564,0.00067251275,0.0011203352,0.0017746455,0.00085051346,0.009871957],"category_scores_gemma":[0.0056977323,0.0005907135,0.0013288587,0.0029330645,0.00026426732,0.0012457139,0.0012462105,0.001169034,0.005866829],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010566474,0.00048280976,0.05317658,0.00055700046,0.00064677605,0.00029709496,0.0005268673,0.06736702,0.02946009,0.007365273,0.0954666,0.7435972],"study_design_scores_gemma":[0.00019951005,0.0001815342,0.028144807,0.000056074834,0.00014963589,0.00044090793,0.00019011238,0.8665517,0.029072398,0.006824437,0.06802884,0.00016000765],"about_ca_topic_score_codex":0.0064516105,"about_ca_topic_score_gemma":0.0100751,"teacher_disagreement_score":0.009871957,"about_ca_system_score_codex":0.0005674474,"about_ca_system_score_gemma":0.0013611595,"threshold_uncertainty_score":0.033024967},"labels":[],"label_agreement":null},{"id":"W2130225077","doi":"10.1086/524980","title":"Evolution of the Bar Fraction in COSMOS: Quantifying the Assembly of the Hubble Sequence","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":420,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Redshift; Bulge; Astronomy; Galaxy; Spiral galaxy; Stellar mass; Universe; Star formation","score_opus":0.024499566978750102,"score_gpt":0.2475264864854448,"score_spread":0.2230269195066947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130225077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987801,0.00016911158,0.0001925968,0.000009520009,0.000001826296,0.0000017688749,0.0004848077,0.000013458374,0.00034698614],"genre_scores_gemma":[0.99859303,0.000045578818,0.00023351592,0.00000486624,0.000004503683,0.000001686504,0.00091345346,0.000006928964,0.00019644463],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997316,0.000055705234,0.000018662902,0.000093333205,0.00004643024,0.000054171156],"domain_scores_gemma":[0.9973387,0.00057306065,0.0009271705,0.00030921237,0.00038732743,0.00046455118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009199542,0.00034482163,0.00027717132,0.00244917,0.00025583585,0.0008687915,0.0003212111,0.00030757763,0.0012041442],"category_scores_gemma":[0.0035966753,0.00022368472,0.00023150998,0.0015735144,0.00033220625,0.0006034341,0.0005266146,0.00028015516,0.00042109436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007203843,0.0000072498915,0.9953818,0.000007189645,0.000042774423,0.000029217064,0.00013055351,0.0002653946,0.0019025964,0.00008576176,0.000052574116,0.002022849],"study_design_scores_gemma":[7.516843e-7,0.000010873912,0.99919826,0.0000017994091,0.0000047773565,0.000029863604,0.000034126646,0.00034634242,0.00018212748,0.00003659349,0.00015178637,0.0000027545022],"about_ca_topic_score_codex":0.00881845,"about_ca_topic_score_gemma":0.009762727,"teacher_disagreement_score":0.00881845,"about_ca_system_score_codex":0.0002855163,"about_ca_system_score_gemma":0.000108424014,"threshold_uncertainty_score":0.017534256},"labels":[],"label_agreement":null},{"id":"W2130225519","doi":"10.1086/427406","title":"Spectrum of Very High Energy Gamma‐Rays from the blazar 1ES 1959+650 during Flaring Activity in 2002","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Blazar; Physics; Flare; Gamma ray; Astrophysics; Spectral index; Cherenkov radiation; Solar flare; Telescope; High energy; Spectral line; Astronomy; Optics; Atomic physics","score_opus":0.0050568582250365285,"score_gpt":0.18427468343813977,"score_spread":0.17921782521310325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130225519","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978957,0.00010756371,0.0001126857,0.000035493587,0.0000065794243,0.0000045302895,0.00038315676,0.00003982713,0.0014144876],"genre_scores_gemma":[0.997855,0.000060757397,0.00016524506,0.000029695828,0.0000105266845,0.0000021712974,0.0013280563,0.000009811256,0.000538762],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999194,0.00000724433,0.000006905669,0.000018448181,0.000027959402,0.000019933224],"domain_scores_gemma":[0.9997769,0.000023241635,0.000072109346,0.000024940913,0.000040630926,0.000062140505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019436043,0.00025740787,0.00028098546,0.0007729653,0.00042207877,0.0005406984,0.0002002371,0.0003602906,0.00095765153],"category_scores_gemma":[0.00038887915,0.0001568462,0.00018663461,0.000606745,0.00018586087,0.00014957032,0.00029929544,0.00030067196,0.00027789528],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00146386,0.0003540539,0.7414038,0.00017596206,0.00037090783,0.008453597,0.0022342561,0.0016879226,0.2108619,0.0006044537,0.0034582438,0.02893112],"study_design_scores_gemma":[0.000009481732,0.0000654539,0.9966397,0.000005939274,0.000025698842,0.00050362863,0.00007582164,0.0002666146,0.0014546042,0.000022055214,0.0009243616,0.00000669846],"about_ca_topic_score_codex":0.006444224,"about_ca_topic_score_gemma":0.017031485,"teacher_disagreement_score":0.006444224,"about_ca_system_score_codex":0.00043244695,"about_ca_system_score_gemma":0.00008794468,"threshold_uncertainty_score":0.012813389},"labels":[],"label_agreement":null},{"id":"W2130229226","doi":"10.1086/345408","title":"Our Sun. V. A Bright Young Sun Consistent with Helioseismology and Warm Temperatures on Ancient Earth and Mars","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Helioseismology; Mars Exploration Program; Solar irradiance; Standard solar model; Solar mass; Solar constant; Solar wind; Coronal mass ejection; Solar cycle","score_opus":0.007126791263407933,"score_gpt":0.20189575227815224,"score_spread":0.1947689610147443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130229226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.932184,0.0003851246,0.021607222,0.00067915383,0.00015016868,0.000030259218,0.003078258,0.0009453441,0.040940482],"genre_scores_gemma":[0.9921293,0.00008195465,0.004274605,0.00006702283,0.00001558025,0.000008149081,0.0008040229,0.00008457311,0.0025346638],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999422,0.000011334344,0.0000024230221,0.000022104083,0.000011922757,0.000010092884],"domain_scores_gemma":[0.9998783,0.000021121192,0.000022064927,0.00003032872,0.000022255661,0.000025952615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018551103,0.00022670333,0.00023007527,0.00013202474,0.0003548632,0.00083004823,0.00030342463,0.00039743318,0.005568211],"category_scores_gemma":[0.0006527133,0.00020650496,0.00033187988,0.00020925846,0.00018327481,0.0005024919,0.0003487241,0.00039734415,0.00089217006],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042418911,0.00013324892,0.31687537,0.00026807506,0.00033219802,0.0007373183,0.00055996433,0.549172,0.023394408,0.040287685,0.017457716,0.050357815],"study_design_scores_gemma":[0.0002511757,0.00045385963,0.28422934,0.00009713919,0.00018199933,0.0014084294,0.0006796746,0.5826432,0.013309694,0.049209137,0.067418315,0.000118023774],"about_ca_topic_score_codex":0.004081963,"about_ca_topic_score_gemma":0.004149598,"teacher_disagreement_score":0.005568211,"about_ca_system_score_codex":0.00031063688,"about_ca_system_score_gemma":0.000255101,"threshold_uncertainty_score":0.018627524},"labels":[],"label_agreement":null},{"id":"W2130527029","doi":"10.1088/0004-637x/773/2/102","title":"<i>HERSCHEL</i>REVEALS MASSIVE COLD CLUMPS IN NGC 7538","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; National Research Council Canada; Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Spire (mollusc); Physics; Astrophysics; Stars; Luminosity; Star formation; High mass; Infrared; Astronomy; Young stellar object; Cover (algebra); Far infrared; Galaxy","score_opus":0.008798438280872274,"score_gpt":0.22763296037761122,"score_spread":0.21883452209673895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130527029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99579465,0.00018828374,0.00012468829,0.000043685093,0.0000022402874,0.0000060198754,0.0010161118,0.000058295165,0.0027660008],"genre_scores_gemma":[0.99751174,0.00009882218,0.00050490483,0.000043537962,0.000008041902,0.000005900787,0.0011824304,0.000012536984,0.0006320498],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991083,0.0000036035885,0.000004418187,0.000022711678,0.000026683474,0.000031779105],"domain_scores_gemma":[0.9998148,0.000014392065,0.00005710675,0.00003485171,0.000016753893,0.00006212178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012481191,0.00018863604,0.00014228877,0.0011695147,0.0003956178,0.0003794869,0.0002925871,0.00021613357,0.0023316306],"category_scores_gemma":[0.00018489665,0.0001183274,0.00011781355,0.00066024356,0.00025015336,0.00020556965,0.00042333073,0.00014852063,0.00053730066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013499982,0.00006450202,0.7926686,0.000096306,0.00006969358,0.0017863442,0.0017673479,0.00096672843,0.17058374,0.00050332653,0.0031658497,0.028192611],"study_design_scores_gemma":[0.0000038561284,0.000014022969,0.9962613,0.000007644804,0.0000060124244,0.0003555246,0.00015651489,0.00013885916,0.0011675503,0.000041163472,0.001843462,0.000004111527],"about_ca_topic_score_codex":0.030528707,"about_ca_topic_score_gemma":0.079308785,"teacher_disagreement_score":0.030528707,"about_ca_system_score_codex":0.0004756475,"about_ca_system_score_gemma":0.00015436088,"threshold_uncertainty_score":0.060701966},"labels":[],"label_agreement":null},{"id":"W2130553508","doi":"10.1088/0004-637x/716/2/1269","title":"ANGULAR MOMENTUM TRANSPORT IN SOLAR-TYPE STARS: TESTING THE TIMESCALE FOR CORE-ENVELOPE COUPLING","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Angular momentum; Stars; Astrophysics; Rotation period; Rotation (mathematics); Radiation zone; Convection zone; Envelope (radar); Astronomy; Classical mechanics; Geometry","score_opus":0.02222336676212916,"score_gpt":0.242115042167121,"score_spread":0.21989167540499183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130553508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992661,0.00006843578,0.00033147063,0.000010762204,0.0000013925129,0.0000022129354,0.000027219872,0.000004867927,0.00028761558],"genre_scores_gemma":[0.99981934,0.000018487597,0.00007231688,0.000003404431,0.0000011078477,0.0000013987516,0.000036946454,0.0000024933017,0.00004462777],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999843,0.000026157237,0.000014325658,0.000054790467,0.000029250328,0.00003253167],"domain_scores_gemma":[0.9982419,0.00077191275,0.00046501734,0.0001798359,0.00008325125,0.0002579531],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077041134,0.00033990704,0.00033490604,0.00036383522,0.0002715077,0.0007224525,0.00046195602,0.00037958552,0.001051952],"category_scores_gemma":[0.0029686578,0.00019243656,0.0003603821,0.00027857118,0.00037959256,0.00092187925,0.00095967646,0.00041736156,0.00018046316],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001864596,0.00017727358,0.822846,0.00012173346,0.00024954564,0.00023748445,0.00045063192,0.014079408,0.14560689,0.001965641,0.00007544459,0.01232538],"study_design_scores_gemma":[0.00005323907,0.00072303595,0.9284166,0.000015594045,0.000096677955,0.00019636215,0.00025401943,0.052260134,0.01586034,0.0018811059,0.00021964543,0.000023163642],"about_ca_topic_score_codex":0.003015937,"about_ca_topic_score_gemma":0.0014981298,"teacher_disagreement_score":0.003015937,"about_ca_system_score_codex":0.00045696052,"about_ca_system_score_gemma":0.00021744716,"threshold_uncertainty_score":0.0059967637},"labels":[],"label_agreement":null},{"id":"W2130582991","doi":"10.1088/0004-637x/757/1/89","title":"TWO MILLISECOND PULSARS DISCOVERED BY THE PALFA SURVEY AND A SHAPIRO DELAY MEASUREMENT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Max-Planck-Gesellschaft; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canarie","keywords":"Millisecond pulsar; Pulsar; Millisecond; Neutron star; Measure (data warehouse); Binary number; Solar mass; Orbital plane; Pulsar planet","score_opus":0.031120756662180726,"score_gpt":0.31656748983896965,"score_spread":0.2854467331767889,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130582991","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939877,0.00028216917,0.00068536255,0.00018724526,0.00003669118,0.000016560865,0.0004920264,0.000043737928,0.004268569],"genre_scores_gemma":[0.99514705,0.00019987705,0.0015614592,0.00011455807,0.000053627246,0.000020518202,0.0014234199,0.000010478732,0.0014690482],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977106,0.000022485374,0.000012446687,0.000060568713,0.00007609091,0.00005748093],"domain_scores_gemma":[0.99910456,0.000112207475,0.00032739193,0.000105328385,0.00016255464,0.00018786539],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031157827,0.0002442291,0.00017240511,0.0015692103,0.0005011117,0.0005376988,0.00030160876,0.00037997053,0.0010245919],"category_scores_gemma":[0.00085229176,0.00018611233,0.00017718994,0.0009982184,0.0003278336,0.0004410849,0.0009003008,0.00043449836,0.00032031813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005182773,0.0001630919,0.9135899,0.00007483987,0.00007484643,0.002948859,0.0009371249,0.00014897162,0.03204099,0.0009257726,0.0015953016,0.046982083],"study_design_scores_gemma":[0.000024338733,0.0001720999,0.98732865,0.000007061069,0.000020571206,0.0020059885,0.00018262008,0.00019200136,0.0019095194,0.00012562131,0.008019849,0.000011630072],"about_ca_topic_score_codex":0.003965512,"about_ca_topic_score_gemma":0.0074712615,"teacher_disagreement_score":0.003965512,"about_ca_system_score_codex":0.00043107005,"about_ca_system_score_gemma":0.0002896708,"threshold_uncertainty_score":0.00788486},"labels":[],"label_agreement":null},{"id":"W2130645390","doi":"10.1086/503098","title":"Discovery of a Low-Eccentricity, High-Inclination Kuiper Belt Object at 58 AU","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Eccentricity (behavior); Astronomy; Astrophysics; Astrobiology","score_opus":0.0038807343510976837,"score_gpt":0.19663924029941254,"score_spread":0.19275850594831487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130645390","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984629,0.00008159511,0.00023220267,0.000032760305,0.0000047359536,0.000002560143,0.000053131476,0.000015519505,0.0011145219],"genre_scores_gemma":[0.9988061,0.00003693232,0.0005819253,0.000017846909,0.000010879467,0.0000018034865,0.00019874428,0.0000025686645,0.00034317738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999515,0.0000032359603,0.0000021035921,0.000017061822,0.000015203345,0.000010808767],"domain_scores_gemma":[0.9998611,0.000015811198,0.00005893787,0.000025539051,0.000010942565,0.000027706783],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009845082,0.00011070245,0.00013767551,0.00030136073,0.0004385384,0.0004093352,0.00034533962,0.00044020347,0.0010530635],"category_scores_gemma":[0.0002487774,0.00013084714,0.00007549755,0.00017790026,0.00030161568,0.00028014474,0.00038944773,0.0003349654,0.00050211244],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044615485,0.00020531236,0.6092707,0.00008354939,0.000065468375,0.00996645,0.0020006537,0.00030349972,0.33735526,0.0013164168,0.00089473184,0.038091782],"study_design_scores_gemma":[0.000028015653,0.00044920907,0.95763534,0.000013901462,0.000041482315,0.009684736,0.00034937458,0.00080041995,0.021133082,0.00033608061,0.009514824,0.000013663744],"about_ca_topic_score_codex":0.00047883237,"about_ca_topic_score_gemma":0.00081239955,"teacher_disagreement_score":0.0010530635,"about_ca_system_score_codex":0.00016167478,"about_ca_system_score_gemma":0.000078542376,"threshold_uncertainty_score":0.003522873},"labels":[],"label_agreement":null},{"id":"W2130843916","doi":"10.1088/0004-637x/691/1/687","title":"THE<i>CHANDRA</i>DEEP PROTOCLUSTER SURVEY: EVIDENCE FOR AN ENHANCEMENT OF AGN ACTIVITY IN THE SSA22 PROTOCLUSTER AT<i>z</i>= 3.09","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Smithsonian Institution","keywords":"Physics; Astrophysics; Supermassive black hole; Active galactic nucleus; Galaxy; Chandra Deep Field South; Population; Accretion (finance); Medicine","score_opus":0.03303340936154328,"score_gpt":0.2938784252035524,"score_spread":0.26084501584200914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130843916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99879503,0.0000930601,0.000096848715,0.00002546821,0.0000021834228,0.000004257858,0.00030351433,0.00002513784,0.00065453764],"genre_scores_gemma":[0.99873656,0.00008588275,0.00024488172,0.00003180824,0.000008797245,0.0000043698747,0.0005818701,0.000009163395,0.00029669204],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999,0.000005702995,0.0000050351887,0.000020445601,0.000030615596,0.000038244027],"domain_scores_gemma":[0.99940455,0.000018439561,0.00023169091,0.00004060882,0.000072001494,0.00023271465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012252518,0.0003085151,0.00027696104,0.0009243442,0.00039605022,0.0007410001,0.0002500134,0.00017828846,0.00089667743],"category_scores_gemma":[0.00030145238,0.00018914575,0.00020347936,0.00060740573,0.00028707733,0.0002864567,0.0007552106,0.00028526626,0.0002784979],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012918473,0.00002636903,0.95542634,0.0000192915,0.00006434561,0.00044720707,0.0004000764,0.00007587826,0.037577663,0.000092434115,0.000422685,0.0053184833],"study_design_scores_gemma":[0.0000029052942,0.000014769281,0.99864,0.0000018288895,0.0000071301365,0.0001752156,0.00006486138,0.000056756024,0.0005839216,0.000010371457,0.00043998563,0.0000022869447],"about_ca_topic_score_codex":0.0104510365,"about_ca_topic_score_gemma":0.022398084,"teacher_disagreement_score":0.0104510365,"about_ca_system_score_codex":0.00034124346,"about_ca_system_score_gemma":0.00018660881,"threshold_uncertainty_score":0.020780444},"labels":[],"label_agreement":null},{"id":"W2130879182","doi":"10.1086/524981","title":"Verifying the Cosmological Utility of Type Ia Supernovae: Implications of a Dispersion in the Ultraviolet Spectra","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":142,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Supernova; Redshift; Galaxy; Metallicity; Cosmology; Extinction (optical mineralogy); Spectral line; Ultraviolet; Wavelength; Astronomy; Optics","score_opus":0.029100334596776235,"score_gpt":0.26892516726691257,"score_spread":0.23982483267013632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2130879182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986753,0.00011359181,0.00038795176,0.00001462631,0.0000022664162,0.0000025475053,0.00018844254,0.000011067368,0.0006041506],"genre_scores_gemma":[0.9989899,0.00006325932,0.00045225208,0.0000062478134,0.000008797748,0.000001638314,0.00035371166,0.0000043446885,0.000119804245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99953187,0.000113239745,0.000052383773,0.00010888747,0.00012781656,0.00006575493],"domain_scores_gemma":[0.9958103,0.0012085461,0.0015120615,0.0006838593,0.00041535913,0.0003699181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011360277,0.00030812382,0.00017928182,0.0014579257,0.00046652797,0.0008316395,0.00035214692,0.00025510663,0.0011094264],"category_scores_gemma":[0.005110307,0.00015331924,0.00029052846,0.0011811706,0.00039811342,0.0004870514,0.0006665355,0.00025085366,0.0002199475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000035058503,0.00001230188,0.9950381,0.0000050844465,0.000028772378,0.000029130366,0.000037710186,0.0002814343,0.0017195395,0.00010168195,0.00003373946,0.0026774888],"study_design_scores_gemma":[0.0000019700637,0.000030185845,0.9969234,0.0000031342174,0.000018114642,0.000095688105,0.00008994983,0.0014557233,0.0010538644,0.00014574449,0.00017865507,0.0000035596715],"about_ca_topic_score_codex":0.0054496443,"about_ca_topic_score_gemma":0.007935937,"teacher_disagreement_score":0.0054496443,"about_ca_system_score_codex":0.00029220962,"about_ca_system_score_gemma":0.00018906369,"threshold_uncertainty_score":0.010835886},"labels":[],"label_agreement":null},{"id":"W2131033902","doi":"10.1088/0004-637x/806/1/38","title":"THE KINEMATIC AND CHEMICAL PROPERTIES OF A POTENTIAL CORE-FORMING CLUMP: PERSEUS B1-E","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Velocity gradient; Kinematics; Line (geometry); James Clerk Maxwell Telescope; Telescope; Radial velocity; Submillimeter Array","score_opus":0.022806332177447954,"score_gpt":0.23343141124989256,"score_spread":0.2106250790724446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131033902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99896264,0.00008946788,0.00010483903,0.00001585041,0.0000021093344,0.000005460892,0.00016564367,0.000016119668,0.0006378408],"genre_scores_gemma":[0.998896,0.000053835945,0.00035374978,0.000020809037,0.00000549124,0.0000036186354,0.00045079057,0.000006826207,0.00020883082],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999356,0.0000025972415,0.0000020814919,0.00002168044,0.000016412127,0.000021568358],"domain_scores_gemma":[0.9996582,0.000023997785,0.000114576054,0.00001849042,0.000044512537,0.0001402564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015396692,0.00039367334,0.00023304053,0.0012895155,0.0005218546,0.00046284834,0.00049728906,0.0003350721,0.0011134774],"category_scores_gemma":[0.0002589624,0.00019984419,0.00009993766,0.00069380313,0.00029110102,0.00024487192,0.0005086925,0.00027015802,0.0004177377],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002594212,0.000061353305,0.9375664,0.00002695662,0.000028653363,0.00062213815,0.00031678673,0.00055731315,0.050953027,0.00014622576,0.00041916684,0.009042674],"study_design_scores_gemma":[0.000015723668,0.000041717347,0.9954085,0.0000071388754,0.000008729175,0.000293746,0.0002124601,0.0011527655,0.0022030363,0.00005727226,0.0005940998,0.000004805643],"about_ca_topic_score_codex":0.011972661,"about_ca_topic_score_gemma":0.015676511,"teacher_disagreement_score":0.011972661,"about_ca_system_score_codex":0.0003888141,"about_ca_system_score_gemma":0.00012328038,"threshold_uncertainty_score":0.023805976},"labels":[],"label_agreement":null},{"id":"W2131293516","doi":"10.1086/507598","title":"Helium‐rich Thermonuclear Bursts and the Distance to the Accretion‐powered Millisecond Pulsar SAX J1808.4−3658","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Thermonuclear fusion; Accretion (finance); Millisecond pulsar; Flux (metallurgy); Neutron star; RADIUS; Helium; Pulsar; White dwarf; Metallicity; Astronomy; Atomic physics; Plasma; Stars; Nuclear physics","score_opus":0.00574467145431454,"score_gpt":0.2061817822133361,"score_spread":0.20043711075902157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131293516","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997609,0.00002112413,0.000020513493,0.0000038218714,6.8159943e-7,5.520329e-7,0.000031719694,0.0000016669854,0.00015904378],"genre_scores_gemma":[0.99957985,0.000027061214,0.00004536536,0.000002350416,0.000004256829,0.0000010460329,0.0001970354,0.0000017681301,0.0001413796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999443,0.0000054648463,0.000006071029,0.000014334259,0.000013733984,0.00001605108],"domain_scores_gemma":[0.9994386,0.000068944835,0.00033606833,0.000032847653,0.00003480512,0.00008871252],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015231656,0.00019752844,0.0001592324,0.00076903094,0.00022642789,0.00045059194,0.00016785556,0.00017390375,0.0008727313],"category_scores_gemma":[0.0006545151,0.00013184597,0.00013366628,0.00037004513,0.00019359674,0.00021408996,0.00033036462,0.00021056419,0.00018303155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024223111,0.00003944179,0.96682054,0.000016557075,0.000046101042,0.0004206695,0.0003092645,0.00074520137,0.026939793,0.0001679088,0.00006870038,0.0041835546],"study_design_scores_gemma":[0.0000039228444,0.000025751446,0.9986884,0.0000021027652,0.000006668727,0.00016275368,0.000048701615,0.00034171538,0.0004706794,0.000039349263,0.00020762763,0.0000024415613],"about_ca_topic_score_codex":0.0021493665,"about_ca_topic_score_gemma":0.0037389568,"teacher_disagreement_score":0.0021493665,"about_ca_system_score_codex":0.00030429836,"about_ca_system_score_gemma":0.000072585,"threshold_uncertainty_score":0.004273653},"labels":[],"label_agreement":null},{"id":"W2131390080","doi":"10.1088/0004-637x/786/1/37","title":"THE Spitzer SURVEY OF INTERSTELLAR CLOUDS IN THE GOULD BELT. VI. THE AURIGA–CALIFORNIA MOLECULAR CLOUD OBSERVED WITH IRAC AND MIPS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Molecular cloud; Young stellar object; Interstellar cloud; Stellar population; Protostar; Population; Cloud computing; Cluster (spacecraft)","score_opus":0.015172670703918912,"score_gpt":0.22588868818209049,"score_spread":0.21071601747817156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131390080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9175006,0.0016595188,0.0009441641,0.00041611757,0.000028447892,0.00013656539,0.061805535,0.00062958983,0.016879493],"genre_scores_gemma":[0.88847625,0.0019332832,0.005748136,0.00024120646,0.000051130777,0.00010398329,0.09358443,0.00013364304,0.009727967],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999031,0.000005771933,0.000005648861,0.000020629363,0.000038157516,0.00002673847],"domain_scores_gemma":[0.99974865,0.000010008526,0.00008704814,0.000028230195,0.00004342997,0.000082774946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016948378,0.00018012295,0.0001513291,0.0024123646,0.0002537939,0.0003046313,0.00028500988,0.000103440194,0.003012965],"category_scores_gemma":[0.0003032488,0.000100574165,0.00011166225,0.0018215221,0.000103686,0.00032579686,0.00054541696,0.00018188765,0.0007454147],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008924844,0.00007678377,0.89219356,0.00009967175,0.00007567233,0.00020001028,0.0005578616,0.00021353125,0.009180875,0.00083616097,0.041322548,0.055154193],"study_design_scores_gemma":[0.0000059326394,0.000007007478,0.98670584,0.000012431629,0.000007892293,0.000042253167,0.00007931534,0.0000966024,0.00022801038,0.00005131122,0.012761689,0.0000017717426],"about_ca_topic_score_codex":0.082742356,"about_ca_topic_score_gemma":0.17273216,"teacher_disagreement_score":0.082742356,"about_ca_system_score_codex":0.0005189122,"about_ca_system_score_gemma":0.0005111709,"threshold_uncertainty_score":0.16452152},"labels":[],"label_agreement":null},{"id":"W2131461871","doi":"10.1088/0004-637x/740/2/86","title":"THE ATACAMA COSMOLOGY TELESCOPE: CALIBRATION WITH THE<i>WILKINSON MICROWAVE ANISOTROPY PROBE</i>USING CROSS-CORRELATIONS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"CMB cold spot; Cosmic microwave background; Physics; Cosmology; Calibration; Multipole expansion; Telescope; Astrophysics; Range (aeronautics); Anisotropy; Noise (video); Remote sensing; Computational physics; Astronomy; Optics; Geology; Computer science","score_opus":0.017333675859434336,"score_gpt":0.23385907329540465,"score_spread":0.21652539743597032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131461871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.63546175,0.001979308,0.21557653,0.0018757654,0.0007919486,0.0002573271,0.011327437,0.007529695,0.1252002],"genre_scores_gemma":[0.87550664,0.00039252653,0.110898,0.00035860503,0.00023446037,0.00015520536,0.004553455,0.0010674227,0.006833877],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99891245,0.00026501718,0.00003584405,0.00029171468,0.00039725742,0.000097750104],"domain_scores_gemma":[0.9980478,0.00014701945,0.00039517845,0.00066906423,0.0005177208,0.00022332885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023858617,0.00039368568,0.0002678008,0.0014921878,0.0007427131,0.0014052725,0.00084402855,0.0005010747,0.0026247518],"category_scores_gemma":[0.0040943627,0.00030304157,0.0003114672,0.0026550046,0.00041936775,0.0013091903,0.0012462556,0.0008840983,0.0019363121],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008111126,0.0002297932,0.4789494,0.00019544558,0.00041344613,0.0002496084,0.0014579858,0.0069481,0.07624096,0.029647155,0.047870472,0.3569865],"study_design_scores_gemma":[0.00022586145,0.00021266604,0.72703844,0.00008890589,0.00020704679,0.0007363008,0.0005474457,0.049356095,0.042945076,0.012241063,0.16621332,0.000187861],"about_ca_topic_score_codex":0.009653066,"about_ca_topic_score_gemma":0.016989235,"teacher_disagreement_score":0.009653066,"about_ca_system_score_codex":0.0006189425,"about_ca_system_score_gemma":0.00096969237,"threshold_uncertainty_score":0.019193769},"labels":[],"label_agreement":null},{"id":"W2131574378","doi":"10.1088/0004-637x/719/1/561","title":"MEASURING THE CLUMP MASS FUNCTION IN THE AGE OF SCUBA2,<i>HERSCHEL</i>, AND ALMA","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Toronto","funders":"","keywords":"Angular resolution (graph drawing); Function (biology); Log-normal distribution; Initial mass function; Red clump; Image resolution; Image (mathematics); Noise (video); Limit (mathematics)","score_opus":0.014585776980887285,"score_gpt":0.2204494752667628,"score_spread":0.20586369828587553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131574378","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99428046,0.00010674275,0.003005913,0.000053746615,0.000008270997,0.000016936172,0.0005146022,0.00021766551,0.0017957302],"genre_scores_gemma":[0.99525356,0.000020303178,0.003977615,0.000021589814,0.0000061394912,0.000008206425,0.00052880426,0.00005252355,0.00013127388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999703,0.00005181021,0.000014230494,0.000086982844,0.00008697886,0.000057002428],"domain_scores_gemma":[0.99817634,0.00042641233,0.00047571547,0.00027535987,0.00036476093,0.00028149656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013733434,0.0003628591,0.00034588922,0.0011728777,0.0004362564,0.0010050453,0.00091324036,0.0006097708,0.00055585755],"category_scores_gemma":[0.003938431,0.0002623506,0.0003683208,0.000838895,0.00041556923,0.0008592616,0.0006009363,0.0005259622,0.00024019381],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080497604,0.00017036346,0.76528436,0.00016596308,0.00031117295,0.0004642779,0.00081174116,0.14168367,0.059924908,0.0051512397,0.0023811676,0.022846138],"study_design_scores_gemma":[0.00007835136,0.00013639344,0.55812126,0.000037428406,0.00007421193,0.00027927756,0.0001458999,0.40947542,0.026990037,0.0016213281,0.002975301,0.00006511936],"about_ca_topic_score_codex":0.009655149,"about_ca_topic_score_gemma":0.012583486,"teacher_disagreement_score":0.009655149,"about_ca_system_score_codex":0.0013587679,"about_ca_system_score_gemma":0.00037337502,"threshold_uncertainty_score":0.019197881},"labels":[],"label_agreement":null},{"id":"W2131882275","doi":"10.1088/0004-637x/770/1/41","title":"SCATTERED EMISSION FROM<i>z</i>∼ 1 GALACTIC OUTFLOWS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Outflow; Galaxy; Redshift; Flux (metallurgy); Emission spectrum; RADIUS; Astronomy; Spectral line","score_opus":0.00755158794817614,"score_gpt":0.2062380911322566,"score_spread":0.19868650318408046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131882275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972402,0.00009130188,0.0011691379,0.0000141949495,0.0000026588777,0.0000047299827,0.00022046194,0.000079650265,0.0011777547],"genre_scores_gemma":[0.9986512,0.00003600218,0.00073960185,0.00001682646,0.0000036478827,0.0000028231805,0.000322557,0.000012114017,0.00021524461],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999498,0.0000035004034,0.0000023518692,0.000021639702,0.0000075821654,0.000014972839],"domain_scores_gemma":[0.99988794,0.0000140608,0.000044331427,0.000015660858,0.000012079498,0.00002599686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011087709,0.00030746273,0.00017437284,0.0002898874,0.0001589989,0.00035382394,0.0002641366,0.00013353024,0.0016299434],"category_scores_gemma":[0.00022256316,0.0001873401,0.00025220236,0.00018906605,0.00013333569,0.00017013095,0.00029158237,0.00021462012,0.00026420888],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032318762,0.00006359561,0.702787,0.00008567099,0.00010903843,0.00047666335,0.00021241257,0.0041363062,0.272681,0.000699424,0.00039717948,0.018028678],"study_design_scores_gemma":[0.000034343433,0.00015830783,0.9666355,0.000017183946,0.000059797505,0.00046638545,0.00009672282,0.0082027735,0.022440955,0.00055236265,0.0013227619,0.00001297043],"about_ca_topic_score_codex":0.0015765656,"about_ca_topic_score_gemma":0.0025496897,"teacher_disagreement_score":0.0016299434,"about_ca_system_score_codex":0.00024150134,"about_ca_system_score_gemma":0.0000625295,"threshold_uncertainty_score":0.0054526925},"labels":[],"label_agreement":null},{"id":"W2131979110","doi":"10.1086/511329","title":"Searching for a Stochastic Background of Gravitational Waves with the Laser Interferometer Gravitational-Wave Observatory","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":147,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Leverhulme Trust; Alexander von Humboldt-Stiftung; Council of Scientific and Industrial Research, India; Alfred P. Sloan Foundation; National Science Foundation; John Simon Guggenheim Memorial Foundation; National Aeronautics and Space Administration","keywords":"LIGO; Gravitational wave; Physics; Interferometry; Observatory; Amplitude; Gravitational wave background; Gravitational-wave observatory; Laser; Limit (mathematics); Optics; Astrophysics; Mathematical analysis; Mathematics","score_opus":0.035875041912195156,"score_gpt":0.329541369690081,"score_spread":0.29366632777788587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131979110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87520283,0.0004516241,0.11499241,0.0016109227,0.000047951475,0.00002721209,0.0006905412,0.00054040086,0.006436183],"genre_scores_gemma":[0.9724062,0.00016201228,0.025932966,0.0001889722,0.000071532704,0.00002234894,0.0008879297,0.000053436826,0.0002745832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982755,0.00045859173,0.00007296841,0.00039849887,0.0006254057,0.00016908257],"domain_scores_gemma":[0.990868,0.0042565637,0.0027921388,0.0009821962,0.0005368921,0.0005643305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0046666684,0.0007097722,0.00071216974,0.0017376348,0.0011245186,0.0027035973,0.00134487,0.0008487048,0.0012645026],"category_scores_gemma":[0.018032236,0.0008322896,0.00051375345,0.0016088822,0.0013901872,0.002124579,0.0030211662,0.0011348223,0.00022734122],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094283134,0.00019871525,0.57457554,0.00018809496,0.00093678327,0.00035807583,0.00057883264,0.11624739,0.057081554,0.16114226,0.0056430004,0.08210692],"study_design_scores_gemma":[0.00026347025,0.00020245208,0.22970457,0.000077380006,0.00025748287,0.0003505604,0.00010072592,0.6103822,0.022919415,0.12646773,0.00911316,0.00016091597],"about_ca_topic_score_codex":0.0032686063,"about_ca_topic_score_gemma":0.005540866,"teacher_disagreement_score":0.0046666684,"about_ca_system_score_codex":0.0013207921,"about_ca_system_score_gemma":0.0008824874,"threshold_uncertainty_score":0.024680018},"labels":[],"label_agreement":null},{"id":"W2131997906","doi":"10.1086/342167","title":"Laboratory Spectroscopy of Hot Water near 2 Microns and Sunspot Spectroscopy in the H‐Band Region","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Spectroscopy; Sunspot; Spectral line; Emission spectrum; Line (geometry); Astrophysics; Infrared spectroscopy; Astronomy; Magnetic field","score_opus":0.00954675289439282,"score_gpt":0.22796586857647932,"score_spread":0.2184191156820865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2131997906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944952,0.00018171246,0.0016828879,0.000022243277,0.000007458542,0.000005873816,0.00018002809,0.00009395902,0.0033305758],"genre_scores_gemma":[0.99704176,0.00009477614,0.0018233219,0.000018455308,0.000008866487,0.0000116974825,0.00021798334,0.000015809119,0.0007671938],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99992025,0.000009484362,0.0000020361265,0.000024083047,0.000022546732,0.00002166599],"domain_scores_gemma":[0.99987817,0.000016937782,0.00003566426,0.000011288713,0.000020286147,0.00003766936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010053283,0.00013242416,0.00013894422,0.0005429317,0.00029206704,0.00023650443,0.00022406144,0.0002083695,0.0024194322],"category_scores_gemma":[0.00016105255,0.000113224436,0.00011863696,0.00039666254,0.00019891608,0.00027886164,0.00042909165,0.00021883968,0.00024915126],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044513767,0.00012167807,0.06451383,0.000084117724,0.000039714057,0.0002478547,0.00032835166,0.00040712496,0.9147699,0.00063838385,0.0007836493,0.017620318],"study_design_scores_gemma":[0.0000918339,0.00080654427,0.54568136,0.000023571585,0.00007013136,0.0010890232,0.0008461487,0.0032502431,0.44077548,0.0007268669,0.0065969783,0.000041745527],"about_ca_topic_score_codex":0.0007821845,"about_ca_topic_score_gemma":0.0013643308,"teacher_disagreement_score":0.0024194322,"about_ca_system_score_codex":0.00015255522,"about_ca_system_score_gemma":0.00009742669,"threshold_uncertainty_score":0.008093834},"labels":[],"label_agreement":null},{"id":"W2132042387","doi":"10.1088/0004-637x/705/1/398","title":"THE SPECTRAL TYPES OF WHITE DWARFS IN MESSIER 4","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"White dwarf; Globular cluster; Stellar classification; Cluster (spacecraft); Context (archaeology); Open cluster; Spectral line; Stars","score_opus":0.007198629334974702,"score_gpt":0.2238614116986761,"score_spread":0.2166627823637014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2132042387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938333,0.00005447436,0.000037483158,0.000016593978,0.000001968603,0.0000013333198,0.00010872385,0.00001167353,0.00038431137],"genre_scores_gemma":[0.9982601,0.000058693233,0.00017991639,0.000025374926,0.000008882886,0.0000032760252,0.00055330986,0.0000065995387,0.0009039067],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998722,0.000008979697,0.0000072940106,0.000052611125,0.000021755633,0.000037134818],"domain_scores_gemma":[0.9997987,0.00001637132,0.0000932112,0.000014232928,0.000016639124,0.000060771046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018081178,0.00033498075,0.00019410539,0.0017557213,0.00042186756,0.00033513023,0.00020051986,0.00015875667,0.0020006143],"category_scores_gemma":[0.00031068482,0.00011646957,0.00018785652,0.00043315862,0.0003081118,0.00023895488,0.0006222818,0.00012324864,0.0004488989],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048626156,0.000024071705,0.9480662,0.000024440871,0.00007019286,0.00043272186,0.0015915502,0.00013047163,0.035456747,0.00022640626,0.0006539952,0.01283694],"study_design_scores_gemma":[0.0000043235245,0.000037843478,0.9972172,0.0000017865982,0.000013473436,0.00017596042,0.00017444215,0.00006843955,0.0012784009,0.000036377445,0.0009870048,0.0000046768737],"about_ca_topic_score_codex":0.004832184,"about_ca_topic_score_gemma":0.013510162,"teacher_disagreement_score":0.004832184,"about_ca_system_score_codex":0.0003782937,"about_ca_system_score_gemma":0.00006772173,"threshold_uncertainty_score":0.00960809},"labels":[],"label_agreement":null},{"id":"W2132092212","doi":"10.1088/0004-637x/756/1/28","title":"<i>SPITZER</i>-IRAC IDENTIFICATION OF<i>HERSCHEL</i>-ATLAS SPIRE SOURCES","year":2012,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"U.S. Department of Energy; U.S. Naval Observatory; Case Western Reserve University; National Science Foundation; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; New Mexico State University; University of Portsmouth; Science and Technology Facilities Council; Universität Basel; University of Pittsburgh; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; Princeton University; Johns Hopkins University; Ohio State University; California Institute of Technology; Jet Propulsion Laboratory; Queen Mary University of London; Drexel University; National Aeronautics and Space Administration","keywords":"Spire (mollusc); Galaxy; Physics; Astrophysics; Redshift; Luminous infrared galaxy; Astronomy; Sky; Population; Star formation","score_opus":0.00913223430393958,"score_gpt":0.22020412467920972,"score_spread":0.21107189037527013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2132092212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93683386,0.00037669268,0.008614284,0.0001644036,0.000024297378,0.00018663706,0.03497621,0.0014956382,0.017327977],"genre_scores_gemma":[0.8963023,0.00025425237,0.02169892,0.00020098311,0.00005918672,0.00022531312,0.0762868,0.00029888705,0.004673285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993598,0.00006221364,0.000039188813,0.00014713903,0.00026511739,0.00012661373],"domain_scores_gemma":[0.99774855,0.00024257277,0.0008720024,0.00048390462,0.00036435152,0.00028865546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013077871,0.00032031906,0.00034510464,0.004277278,0.00050357555,0.00076288177,0.000601313,0.0002682431,0.005314569],"category_scores_gemma":[0.002342693,0.00018982997,0.0004026531,0.0021270653,0.00028292742,0.00043073547,0.0011990926,0.00025681758,0.0038602578],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008709477,0.00006153444,0.9395931,0.00010258983,0.000093610644,0.0002686602,0.00032385718,0.001641763,0.019692488,0.0012059901,0.012903095,0.02402625],"study_design_scores_gemma":[0.0000087153385,0.000026194572,0.98912,0.000016765198,0.000015789179,0.00018278537,0.000087240245,0.0010944159,0.0025741644,0.00019418214,0.006664193,0.000015513497],"about_ca_topic_score_codex":0.0043740226,"about_ca_topic_score_gemma":0.0076948754,"teacher_disagreement_score":0.005314569,"about_ca_system_score_codex":0.00043700685,"about_ca_system_score_gemma":0.00036845755,"threshold_uncertainty_score":0.017778993},"labels":[],"label_agreement":null},{"id":"W2132484295","doi":"10.1088/0004-637x/780/1/44","title":"THE ULTRAVIOLET-BRIGHT, SLOWLY DECLINING TRANSIENT PS1-11af AS A PARTIAL TIDAL DISRUPTION EVENT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":204,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Australian Research Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Queen's University; Ministerio de Ciencia, Tecnología e Innovación Productiva; Queen's University Belfast; Space Telescope Science Institute; Comisión Nacional de Investigación Científica y Tecnológica; Associated Universities; University of Arizona; University of Edinburgh; European Commission; Johns Hopkins University; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; Light curve; Supernova; Redshift; Photosphere; Galaxy; Luminosity; Ejecta; Active galactic nucleus; Flare; Astronomy; Black-body radiation; Spectral line; Radiation","score_opus":0.008942155202586233,"score_gpt":0.24672685948389628,"score_spread":0.23778470428131004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2132484295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964675,0.0004679486,0.00065007264,0.000088879526,0.000011423741,0.000011068575,0.00035182585,0.00008952956,0.001861859],"genre_scores_gemma":[0.9980337,0.0002489072,0.0003080493,0.000048735546,0.000023340124,0.0000053631575,0.0007555789,0.000007973709,0.00056829886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993813,0.000004065723,0.0000034467848,0.000024664736,0.0000119355645,0.000017706398],"domain_scores_gemma":[0.99980134,0.000016130265,0.0000856995,0.00002559077,0.000021351445,0.000049915383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012590518,0.00024851924,0.00021069674,0.0007216762,0.0003624121,0.0006114813,0.00024728663,0.00033841745,0.00079806044],"category_scores_gemma":[0.0002762024,0.00011059874,0.00019591926,0.0004671739,0.0002411737,0.00028679665,0.0003963231,0.00026168983,0.0002754587],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075752736,0.00009342325,0.80205774,0.0002080774,0.00011169821,0.01204514,0.0005973713,0.0009039288,0.13295136,0.0016733134,0.0022954727,0.04630494],"study_design_scores_gemma":[0.00001391039,0.00028696735,0.9524958,0.000028686954,0.00007387319,0.025551157,0.00025797315,0.0015682364,0.00926879,0.000624098,0.009810232,0.000020299693],"about_ca_topic_score_codex":0.0014206817,"about_ca_topic_score_gemma":0.0012261015,"teacher_disagreement_score":0.0014206817,"about_ca_system_score_codex":0.00026714613,"about_ca_system_score_gemma":0.00009023693,"threshold_uncertainty_score":0.002824843},"labels":[],"label_agreement":null},{"id":"W2132856166","doi":"10.1088/0004-637x/743/1/28","title":"A MEASUREMENT OF THE DAMPING TAIL OF THE COSMIC MICROWAVE BACKGROUND POWER SPECTRUM WITH THE SOUTH POLE TELESCOPE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":506,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; University of Chicago; Fermilab; McGill University; U.S. Department of Energy; Gordon and Betty Moore Foundation; National Science Foundation; Yale University; Office of Science; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Physics; CMB cold spot; Cosmic microwave background; Astrophysics; Neutrino; Spectral index; South Pole Telescope; Spectral density; Cosmic background radiation; Reionization; Planck; Amplitude; Anisotropy; Spectral line; Astronomy; Particle physics; Redshift; Galaxy; Quantum mechanics","score_opus":0.016704480212163236,"score_gpt":0.2109699248494019,"score_spread":0.1942654446372387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2132856166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9733277,0.00022321458,0.011974628,0.00022643086,0.00002304899,0.000024549423,0.0027512033,0.00033712207,0.011112119],"genre_scores_gemma":[0.98754126,0.00015205251,0.0080326665,0.000052651478,0.00004656333,0.000026513431,0.0030503175,0.000042186704,0.0010557647],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996996,0.00003628331,0.000007918986,0.00008333792,0.00014395465,0.000028974402],"domain_scores_gemma":[0.99929667,0.00012488311,0.00023940325,0.00013504976,0.00010032899,0.00010363883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040613458,0.00030675766,0.00014244381,0.000980706,0.00020100415,0.00034404208,0.00030702158,0.00027469813,0.0016147301],"category_scores_gemma":[0.0014391163,0.00020916291,0.00020069469,0.0010030722,0.00022356598,0.00042352328,0.0004277289,0.00035613446,0.0005064621],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035682612,0.00007399764,0.82290095,0.00009612641,0.00015618608,0.00032654987,0.0005810221,0.003188716,0.09766348,0.00432441,0.0054054637,0.06492619],"study_design_scores_gemma":[0.000020654981,0.00008859243,0.979387,0.000009620695,0.000034260374,0.0003148306,0.00004188256,0.0067254263,0.0062674535,0.00073011196,0.0063606114,0.00001952734],"about_ca_topic_score_codex":0.002657689,"about_ca_topic_score_gemma":0.0052700834,"teacher_disagreement_score":0.002657689,"about_ca_system_score_codex":0.0002864253,"about_ca_system_score_gemma":0.00013111303,"threshold_uncertainty_score":0.00540179},"labels":[],"label_agreement":null},{"id":"W2132870815","doi":"10.1088/0004-637x/792/2/119","title":"WIDE COOL AND ULTRACOOL COMPANIONS TO NEARBY STARS FROM Pan-STARRS 1","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Air Force Research Laboratory; U.S. Naval Observatory; Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; University of California, Los Angeles; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; California Institute of Technology; Eötvös Loránd Tudományegyetem; National Central University; Space Telescope Science Institute; Queen's University Belfast; National Aeronautics and Space Administration; Queen's University; Johns Hopkins University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Stars; Brown dwarf; Proper motion; Stellar classification; White dwarf; Population; K-type main-sequence star","score_opus":0.008881472858905962,"score_gpt":0.21727453885192044,"score_spread":0.2083930659930145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2132870815","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989201,0.00021549175,0.00016912093,0.000012832203,0.0000021014587,0.000002541291,0.000108067106,0.000016625721,0.0005531448],"genre_scores_gemma":[0.9985056,0.0001321874,0.0004530388,0.000018734363,0.000009888315,0.0000023006712,0.0005935001,0.000004705681,0.00028004334],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999796,0.00001019318,0.000014571955,0.00007410116,0.00006197515,0.00004321165],"domain_scores_gemma":[0.99931276,0.00010951212,0.00029660342,0.00007001987,0.00004377814,0.00016736373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025442164,0.00019948171,0.00029048388,0.0009605762,0.00075510156,0.0006820139,0.00027721492,0.0002548951,0.0012953522],"category_scores_gemma":[0.0006826548,0.00014548044,0.00015003685,0.00078092323,0.00027180687,0.0003637147,0.0011680875,0.0002900718,0.00047114317],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014657032,0.000038912527,0.953786,0.00005073379,0.000029155064,0.0015275353,0.000700762,0.00014188616,0.02209676,0.00029744575,0.00034461837,0.020839632],"study_design_scores_gemma":[0.000007644481,0.00015271301,0.9873661,0.00001106473,0.000024479046,0.0045133787,0.00037497294,0.00047269743,0.0035797132,0.00026356863,0.0032256676,0.000008042272],"about_ca_topic_score_codex":0.0010908216,"about_ca_topic_score_gemma":0.0033851296,"teacher_disagreement_score":0.0012953522,"about_ca_system_score_codex":0.00017447161,"about_ca_system_score_gemma":0.00016741616,"threshold_uncertainty_score":0.004333377},"labels":[],"label_agreement":null},{"id":"W2133065879","doi":"10.1088/0004-637x/767/2/126","title":"THE HERSCHEL AND JCMT GOULD BELT SURVEYS: CONSTRAINING DUST PROPERTIES IN THE PERSEUS B1 CLUMP WITH PACS, SPIRE, AND SCUBA-2","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; National Research Council Canada; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"James Clerk Maxwell Telescope; Protein filament; Wavelength; Star formation; Data reduction; Protostar; Infrared","score_opus":0.017489688103865964,"score_gpt":0.21865695470136717,"score_spread":0.2011672665975012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133065879","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98889905,0.00048438908,0.0009382402,0.00020831605,0.000019587715,0.000030187884,0.0064652474,0.00027250784,0.0026825385],"genre_scores_gemma":[0.98518604,0.0001964586,0.004399994,0.00013121043,0.000047206846,0.00003703061,0.009428633,0.00007810024,0.00049539394],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969757,0.00004323015,0.000012771742,0.000092813,0.000093106806,0.000060624996],"domain_scores_gemma":[0.99898463,0.00010259002,0.00036024212,0.00018897573,0.00012382628,0.00023971271],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078078476,0.00047470763,0.0002167686,0.0024607575,0.00033883017,0.00056972133,0.0005524239,0.0003226945,0.001151291],"category_scores_gemma":[0.0013485767,0.00023562978,0.00020634044,0.0014225297,0.0002571263,0.00034067204,0.00083345943,0.00023157445,0.0005898021],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013309416,0.000054842945,0.95551634,0.0000495589,0.000088936235,0.00026285255,0.00023621526,0.0017794552,0.010068599,0.00039831345,0.005486207,0.025925564],"study_design_scores_gemma":[0.000041198582,0.000011940951,0.9938148,0.000012548833,0.000014923585,0.00007100746,0.00005935051,0.0024465797,0.0009721911,0.00012709264,0.0024200224,0.000008327943],"about_ca_topic_score_codex":0.040854786,"about_ca_topic_score_gemma":0.06326836,"teacher_disagreement_score":0.040854786,"about_ca_system_score_codex":0.00072060863,"about_ca_system_score_gemma":0.00042908578,"threshold_uncertainty_score":0.08123398},"labels":[],"label_agreement":null},{"id":"W2133224477","doi":"10.1086/377168","title":"Angular Clustering with Photometric Redshifts in the Sloan Digital Sky Survey: Bimodality in the Clustering Properties of Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Apache (Canada)","funders":"","keywords":"Astrophysics; Physics; Redshift; Galaxy; Cluster analysis; Sky; Luminosity; Redshift survey; Astronomy; Luminosity function; Statistics; Mathematics","score_opus":0.01726206561024438,"score_gpt":0.21436700517090881,"score_spread":0.19710493956066444,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133224477","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99663925,0.00018073274,0.0017369001,0.00006686014,0.000001801583,0.0000048122,0.00040405628,0.000100180776,0.00086534774],"genre_scores_gemma":[0.9988456,0.000041876607,0.00046886163,0.000010839888,0.0000041097414,0.000004510991,0.00046174688,0.000011272065,0.00015114064],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994055,0.00017190358,0.00003170582,0.00014930713,0.00012537024,0.00011628173],"domain_scores_gemma":[0.9948626,0.001727691,0.0017746328,0.00068058737,0.00046113494,0.0004933658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012098823,0.00025492354,0.00027743835,0.003128582,0.00030217378,0.0007385278,0.00031592476,0.00032328514,0.0008485767],"category_scores_gemma":[0.005046755,0.0002508919,0.000324127,0.0025269361,0.00080745015,0.0005727657,0.0009072384,0.00040809234,0.00032920792],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008146415,0.000018393763,0.9829548,0.000015542873,0.000057130772,0.00006248957,0.0002524228,0.0064842724,0.0018962229,0.0005131294,0.0005993123,0.007064855],"study_design_scores_gemma":[0.0000028020334,0.000007753806,0.9860663,0.0000049040136,0.000011357276,0.000053069725,0.00008170012,0.012821062,0.0003233359,0.00040604014,0.00021127574,0.000010489149],"about_ca_topic_score_codex":0.02120996,"about_ca_topic_score_gemma":0.016000578,"teacher_disagreement_score":0.02120996,"about_ca_system_score_codex":0.0007089596,"about_ca_system_score_gemma":0.00025432633,"threshold_uncertainty_score":0.042173028},"labels":[],"label_agreement":null},{"id":"W2133236236","doi":"10.1088/0004-637x/781/2/117","title":"SEARCHING FOR PULSARS USING IMAGE PATTERN RECOGNITION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia; University of British Columbia Hospital","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Artificial intelligence; Set (abstract data type); Noise (video); Pattern recognition (psychology); Computer science; Data set; Artificial neural network; Physics; Test set; Salient; Image (mathematics); Astrophysics","score_opus":0.028223564838952924,"score_gpt":0.3476009768078635,"score_spread":0.31937741196891056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133236236","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.10164501,0.0013066479,0.87257576,0.00092407595,0.00022515946,0.00023959688,0.0010906524,0.010073245,0.0119198775],"genre_scores_gemma":[0.3766799,0.0010109616,0.61044633,0.0005596977,0.00017448835,0.00015951369,0.003287039,0.00032974896,0.007352269],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996575,0.000028883742,0.000022333405,0.00013049047,0.00012144759,0.00003941454],"domain_scores_gemma":[0.99959964,0.00011061782,0.000080885045,0.000067768764,0.00010890254,0.00003215471],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036150182,0.00076929847,0.00056047615,0.002795166,0.00031537557,0.0011944142,0.0009508794,0.0006673485,0.0029760723],"category_scores_gemma":[0.0010983784,0.00026468188,0.00063695904,0.001569759,0.00043642402,0.0013163903,0.0008779195,0.00059395353,0.0019771021],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013753143,0.000105630475,0.0077294214,0.00014025082,0.000069037655,0.00019899204,0.000083211555,0.014532235,0.034101255,0.0024075895,0.0063031428,0.9341918],"study_design_scores_gemma":[0.000045123485,0.00027569456,0.01870911,0.00007703233,0.00009125458,0.0007808251,0.00028281554,0.8733089,0.0624577,0.016158696,0.027751314,0.00006155415],"about_ca_topic_score_codex":0.0018732491,"about_ca_topic_score_gemma":0.0017806032,"teacher_disagreement_score":0.0029760723,"about_ca_system_score_codex":0.00036171539,"about_ca_system_score_gemma":0.00033440065,"threshold_uncertainty_score":0.009955883},"labels":[],"label_agreement":null},{"id":"W2133296000","doi":"10.1086/514809","title":"350 μm Observations of Ultraluminous Infrared Galaxies at Intermediate Redshifts","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Redshift; Galaxy; Luminous infrared galaxy; Star formation; Luminosity; Astronomy; Infrared; Far infrared; Flux (metallurgy); Emissivity; Optics","score_opus":0.012842015406593403,"score_gpt":0.22277632806241995,"score_spread":0.20993431265582654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133296000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99803644,0.0001893149,0.00036865662,0.000011129328,0.0000017686708,0.0000059916274,0.0003252339,0.00006284686,0.0009987247],"genre_scores_gemma":[0.9980081,0.00007657146,0.00095094496,0.000025976706,0.000006586029,0.000005627487,0.00069510273,0.000005178532,0.00022589247],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983966,0.000011978951,0.000006603945,0.00004790904,0.00003529348,0.000058538997],"domain_scores_gemma":[0.99968016,0.000036311336,0.000105508734,0.000031799056,0.000025245852,0.00012101425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028993853,0.0002424098,0.00023036763,0.0013764958,0.00025750927,0.00037790244,0.00037850617,0.0002054515,0.0006096358],"category_scores_gemma":[0.0003655475,0.00017105356,0.00025025784,0.0007279467,0.00018915116,0.00023562774,0.00040876493,0.000238846,0.00017491102],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000222197,0.00010199558,0.950582,0.000037578367,0.00009036247,0.00024080921,0.00062526297,0.0005068803,0.025273973,0.000310265,0.00056749466,0.0214411],"study_design_scores_gemma":[0.0000038080977,0.000032249405,0.9986291,0.0000031723196,0.000014063135,0.000074490395,0.000040913743,0.00018762205,0.00051122584,0.000029944527,0.00047070038,0.000002800048],"about_ca_topic_score_codex":0.005228923,"about_ca_topic_score_gemma":0.009907971,"teacher_disagreement_score":0.005228923,"about_ca_system_score_codex":0.00039110854,"about_ca_system_score_gemma":0.0000884768,"threshold_uncertainty_score":0.010397017},"labels":[],"label_agreement":null},{"id":"W2133385779","doi":"10.1088/0004-637x/692/1/81","title":"TESTING MASS LOSS IN LARGE MAGELLANIC CLOUD CEPHEIDS USING INFRARED AND OPTICAL OBSERVATIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cepheid variable; Metallicity; Physics; Astrophysics; Large Magellanic Cloud; Infrared; Luminosity; Astronomy; Stars; Galaxy","score_opus":0.028035357198576045,"score_gpt":0.25990623777788424,"score_spread":0.2318708805793082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133385779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99811614,0.000057284735,0.00089795963,0.000011854632,0.0000014506928,0.000005713892,0.0001424574,0.000021795959,0.000745436],"genre_scores_gemma":[0.9993562,0.000017051176,0.0003070426,0.0000051171437,0.0000018406352,0.0000027341086,0.00019726015,0.000004377635,0.00010845197],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99948776,0.00011994582,0.000026793898,0.0001576413,0.00014451845,0.000063337226],"domain_scores_gemma":[0.99686027,0.0015463121,0.00080720725,0.000275375,0.00027584995,0.00023497063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010684122,0.0004564153,0.0002502211,0.0010544227,0.0003394029,0.0007910682,0.00058334967,0.00038380237,0.0009613402],"category_scores_gemma":[0.0040831277,0.00020126748,0.00027868967,0.0007565536,0.0003479198,0.00084165327,0.00058459,0.0002466784,0.0003727715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023914517,0.000052916723,0.986206,0.000013424279,0.000052687,0.00013442106,0.0001375202,0.004361866,0.0039368365,0.00014613841,0.000057346308,0.004661586],"study_design_scores_gemma":[0.000008750215,0.00011250815,0.9749761,0.000004249732,0.000020437306,0.000096060205,0.00015448274,0.022146625,0.0021199961,0.000115319526,0.0002395301,0.0000058869714],"about_ca_topic_score_codex":0.00833458,"about_ca_topic_score_gemma":0.005861581,"teacher_disagreement_score":0.00833458,"about_ca_system_score_codex":0.0005951466,"about_ca_system_score_gemma":0.00018363989,"threshold_uncertainty_score":0.016572118},"labels":[],"label_agreement":null},{"id":"W2133493128","doi":"10.1088/0004-637x/787/1/5","title":"DISCOVERY OF A WIDE PLANETARY-MASS COMPANION TO THE YOUNG M3 STAR GU PSC","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Université du Québec à Montréal","funders":"","keywords":"Photometry (optics); Planet; Physics; Brown dwarf; Astronomy; Telescope; Planetary mass; Astrophysics; Near-infrared spectroscopy; Planetary system; Stars","score_opus":0.008272192195799086,"score_gpt":0.2088619005797525,"score_spread":0.20058970838395343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133493128","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983103,0.00025104743,0.00027132066,0.000070541435,0.000008343178,0.0000045901465,0.00005361573,0.000022388354,0.001007895],"genre_scores_gemma":[0.9992137,0.00008926721,0.00037816487,0.00004682822,0.000012039126,0.0000017541475,0.000096380594,0.0000024543065,0.00015931777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995136,0.0000036255828,0.0000030298022,0.000014405003,0.0000143508005,0.000013358251],"domain_scores_gemma":[0.9998147,0.000027162629,0.000058062386,0.000022667755,0.000012182683,0.00006526194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010444384,0.00013583853,0.00016548796,0.00046836934,0.0007049684,0.00046934548,0.00023996607,0.00060157897,0.00067927164],"category_scores_gemma":[0.00042414828,0.00010305455,0.00012922344,0.00040244224,0.00031875962,0.00028853878,0.0007401271,0.0003638772,0.0002821056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046966536,0.00012961286,0.74166054,0.0001687299,0.00006053192,0.05962557,0.0015354836,0.00044213873,0.15007222,0.0015257265,0.0017654358,0.042544387],"study_design_scores_gemma":[0.000022477036,0.00054910994,0.8904232,0.000025909105,0.00005336435,0.08380073,0.0005536661,0.0012954838,0.013630743,0.0012624621,0.008362135,0.000020736457],"about_ca_topic_score_codex":0.00082712696,"about_ca_topic_score_gemma":0.0010176242,"teacher_disagreement_score":0.00082712696,"about_ca_system_score_codex":0.00020614966,"about_ca_system_score_gemma":0.00015873744,"threshold_uncertainty_score":0.002272427},"labels":[],"label_agreement":null},{"id":"W2133526479","doi":"10.1086/508403","title":"A Survey of 56 Midlatitude EGRET Error Boxes for Radio Pulsars","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Egret; Astrophysics; Physics; Luminosity; Millisecond pulsar; Population; Astronomy; Radio telescope; Green Bank Telescope; Galaxy; Gamma ray","score_opus":0.015936071314280424,"score_gpt":0.25092981468497183,"score_spread":0.2349937433706914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133526479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969976,0.00025600797,0.0011021009,0.000029178716,0.0000039154825,0.00001093066,0.0008835106,0.000087515655,0.00062914897],"genre_scores_gemma":[0.9907919,0.00024953866,0.002874211,0.00004431923,0.000014315669,0.00003702233,0.0051521915,0.00007026857,0.0007663663],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989913,0.00020471631,0.0001733003,0.00022167794,0.00028664773,0.00012240303],"domain_scores_gemma":[0.99348736,0.0013487865,0.0027023752,0.001111956,0.0009841481,0.00036531346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018066276,0.00043450395,0.00039127993,0.0027150318,0.00039471145,0.00095604884,0.0006751997,0.0002618823,0.0015332585],"category_scores_gemma":[0.006226554,0.00021525868,0.00020829162,0.0018516162,0.00026497172,0.00064539857,0.0010607338,0.00024748262,0.0009014674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014902493,0.000029103672,0.9775645,0.000021397394,0.000036752266,0.000073879215,0.00047016933,0.00013781265,0.0024793237,0.00012961989,0.0003669968,0.018541334],"study_design_scores_gemma":[0.0000057985926,0.000043149033,0.99572563,0.000013163189,0.000016513235,0.00020590927,0.00019391204,0.0004528706,0.0010168698,0.000045884753,0.0022736609,0.0000065685986],"about_ca_topic_score_codex":0.0023948173,"about_ca_topic_score_gemma":0.0027089254,"teacher_disagreement_score":0.0027150318,"about_ca_system_score_codex":0.00029965834,"about_ca_system_score_gemma":0.0002153476,"threshold_uncertainty_score":0.009554505},"labels":[],"label_agreement":null},{"id":"W2133768772","doi":"10.1086/375734","title":"Detection of Dark Matter Skewness in the VIRMOS‐DESCART Survey: Implications for Ω<sub>0</sub>","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Skewness; Physics; Weak gravitational lensing; Gravitational lens; Dark matter; Measure (data warehouse); Astrophysics; Gaussian; Statistical physics; Statistics; Galaxy; Redshift; Quantum mechanics; Mathematics","score_opus":0.010849318772749762,"score_gpt":0.22460151912054774,"score_spread":0.213752200347798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133768772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99735415,0.000052877764,0.0013834276,0.0001100112,0.0000035429846,0.000003053632,0.00024392533,0.00007261809,0.000776422],"genre_scores_gemma":[0.9986066,0.000030370733,0.0008700183,0.000022209999,0.000003611045,0.0000025656839,0.00037144648,0.000013705804,0.00007948277],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979824,0.00006248914,0.000012810894,0.000033989825,0.000049657363,0.000042865373],"domain_scores_gemma":[0.9984402,0.0003675845,0.0004213324,0.0002698463,0.00020968767,0.000291303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010332016,0.00022012563,0.0002156112,0.00039652077,0.00026300928,0.0006749208,0.00025963335,0.00017041068,0.00060531544],"category_scores_gemma":[0.002383542,0.00018501833,0.00028998443,0.0006471999,0.00043466053,0.00042790323,0.00050406705,0.0002127743,0.00018302421],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013670143,0.00001701672,0.9808543,0.0000132546065,0.0000527395,0.00015560647,0.00011142764,0.0032028726,0.008566935,0.0008694739,0.0003670779,0.0056526624],"study_design_scores_gemma":[0.000009470924,0.00001675221,0.9740457,0.000008175042,0.0000127347275,0.000116902294,0.00008924264,0.021351378,0.0028969503,0.00080833194,0.0006243521,0.000019999738],"about_ca_topic_score_codex":0.020922013,"about_ca_topic_score_gemma":0.023212964,"teacher_disagreement_score":0.020922013,"about_ca_system_score_codex":0.0006430375,"about_ca_system_score_gemma":0.00042262208,"threshold_uncertainty_score":0.041600466},"labels":[],"label_agreement":null},{"id":"W2133991519","doi":"10.1086/589963","title":"The Mass Distribution and Lifetime of Prestellar Cores in Perseus, Serpens, and Ophiuchus","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":319,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"University of Texas at Austin; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Ophiuchus; Serpens; Protostar; Astrophysics; Physics; Star formation; Molecular cloud; Core (optical fiber); Stellar mass; Astronomy; Stars; Optics","score_opus":0.007620176977640571,"score_gpt":0.21439145681299607,"score_spread":0.2067712798353555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2133991519","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996407,0.000056072022,0.000022419516,0.000003869777,2.6233647e-7,7.3677444e-7,0.00011752376,0.0000023272567,0.00015607679],"genre_scores_gemma":[0.9993537,0.00005392095,0.00006251231,0.0000062546615,0.0000013983454,0.0000015259857,0.00038867278,0.000001446608,0.00013061127],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999323,0.0000073483097,0.0000058083256,0.000022904733,0.000011487429,0.000020128273],"domain_scores_gemma":[0.99952924,0.00005846019,0.00021224299,0.000032301934,0.000052602856,0.00011523043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012700415,0.00017539736,0.00011021004,0.0019977991,0.0001966938,0.00032441484,0.00025315324,0.00012674948,0.0007779703],"category_scores_gemma":[0.000613369,0.00008916702,0.00010257942,0.0005420072,0.00030172238,0.00028277934,0.0003728276,0.00007990889,0.0002146811],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000058302903,0.0000073922133,0.99097085,0.000005480256,0.00001506416,0.00008816852,0.00032880894,0.00013552651,0.003797357,0.000062665655,0.00008285549,0.004447563],"study_design_scores_gemma":[0.0000017297449,0.000011480865,0.9990312,0.0000017762463,0.0000032497894,0.00010409789,0.0001474027,0.0001699281,0.00033257582,0.000031984404,0.00016314512,0.0000014154651],"about_ca_topic_score_codex":0.010998131,"about_ca_topic_score_gemma":0.01685067,"teacher_disagreement_score":0.010998131,"about_ca_system_score_codex":0.00033135884,"about_ca_system_score_gemma":0.00011272039,"threshold_uncertainty_score":0.021868229},"labels":[],"label_agreement":null},{"id":"W2134058281","doi":"10.1086/520504","title":"Breathing in Low‐Mass Galaxies: A Study of Episodic Star Formation","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":167,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Star formation; Dwarf galaxy; Virial theorem; Supernova; Galaxy; Halo; Astronomy; RADIUS; Stars; Local Group; Dwarf spheroidal galaxy; Lenticular galaxy","score_opus":0.008086489164807578,"score_gpt":0.22592991133599466,"score_spread":0.21784342217118707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2134058281","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99669856,0.000091115595,0.0016153237,0.0001478512,0.000009799455,0.000013802509,0.00007503131,0.000054628887,0.0012939391],"genre_scores_gemma":[0.9987373,0.00004637318,0.0007634734,0.000042436328,0.00000833359,0.000010441626,0.00012421046,0.000018624029,0.00024881773],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99986255,0.00004563885,0.0000070490632,0.000025654648,0.000018402432,0.000040711097],"domain_scores_gemma":[0.99859184,0.0006407644,0.00019227112,0.00009669945,0.00009751616,0.00038094126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005780441,0.00047948593,0.00060681615,0.00056360685,0.0006847613,0.0007930721,0.0013999309,0.0012175698,0.0010562108],"category_scores_gemma":[0.0033252933,0.00037878158,0.0005545602,0.0005088644,0.0010664292,0.0007918069,0.0009234177,0.0009105166,0.00016023597],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002199585,0.00028302308,0.06779108,0.000043800683,0.00013866035,0.0004121594,0.0003756447,0.9187496,0.0029827727,0.0044432837,0.00082742155,0.0037325625],"study_design_scores_gemma":[0.000059986036,0.000068987494,0.009416882,0.0000074117065,0.000015177625,0.000039014045,0.00009331168,0.98805434,0.00024884893,0.001719346,0.0002656084,0.0000110582905],"about_ca_topic_score_codex":0.022307703,"about_ca_topic_score_gemma":0.011550711,"teacher_disagreement_score":0.022307703,"about_ca_system_score_codex":0.0011348181,"about_ca_system_score_gemma":0.0005385895,"threshold_uncertainty_score":0.04435569},"labels":[],"label_agreement":null},{"id":"W2134149277","doi":"10.1088/0004-637x/737/2/74","title":"SUNYAEV-ZEL'DOVICH EFFECT OBSERVATIONS OF STRONG LENSING GALAXY CLUSTERS: PROBING THE OVERCONCENTRATION PROBLEM","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Sunyaev–Zel'dovich effect; Physics; Weak gravitational lensing; Galaxy cluster; Astrophysics; Scaling; Strong gravitational lensing; Gravitational lens; Monte Carlo method; RADIUS; Galaxy; Statistics; Redshift","score_opus":0.02076361166417997,"score_gpt":0.21857321446139213,"score_spread":0.19780960279721216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2134149277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98915267,0.0007687832,0.0014925548,0.000506096,0.000014749963,0.000006614848,0.00020413884,0.00006583987,0.0077886498],"genre_scores_gemma":[0.9991689,0.00011580019,0.00013009785,0.000034949207,0.000008222563,0.0000018383184,0.00005190223,0.000006294575,0.00048200847],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968934,0.000057465928,0.000016947284,0.00008458471,0.00007393598,0.00007776704],"domain_scores_gemma":[0.9980738,0.0006548502,0.00049854355,0.0003007229,0.00014889445,0.000323161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072435796,0.00015391069,0.0003395576,0.0009962252,0.00075495866,0.0010099775,0.0003649077,0.00032599695,0.00252499],"category_scores_gemma":[0.0029953583,0.00021316358,0.00019429057,0.00094354997,0.0009996283,0.0008262678,0.0012969774,0.00037290514,0.00019696103],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043481652,0.00006148268,0.9071617,0.00009125761,0.00022084902,0.00022251067,0.0011429269,0.0030210745,0.014585825,0.018358551,0.0038642967,0.050834626],"study_design_scores_gemma":[0.00006372562,0.000053576496,0.9796816,0.000017523493,0.0000751016,0.00014381402,0.0007402916,0.0036048663,0.0028181074,0.007572883,0.005204386,0.000024084718],"about_ca_topic_score_codex":0.016362207,"about_ca_topic_score_gemma":0.017829414,"teacher_disagreement_score":0.016362207,"about_ca_system_score_codex":0.00070312864,"about_ca_system_score_gemma":0.0004911272,"threshold_uncertainty_score":0.032533944},"labels":[],"label_agreement":null},{"id":"W2134425851","doi":"10.1086/424998","title":"The Double Pulsar System J0737-3039: Modulation of the Radio Emission from B by Radiation from A","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Radiation; Telescope; Line-of-sight; Radio telescope; Pulse (music); Green Bank Telescope; Modulation (music); Electromagnetic radiation","score_opus":0.0073449925653345126,"score_gpt":0.2690560754399263,"score_spread":0.2617110828745918,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2134425851","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989373,0.00014658898,0.00015885563,0.000016064334,0.0000067510514,0.0000049268865,0.00019383582,0.000015627791,0.0005200896],"genre_scores_gemma":[0.99820673,0.0000715791,0.0005902866,0.00003051619,0.0000123180325,0.000010256914,0.0008209207,0.000012898517,0.00024439613],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999014,0.000005882622,0.000005236185,0.000027860046,0.000026863436,0.000032796364],"domain_scores_gemma":[0.99972445,0.000034062465,0.000068256064,0.00003596753,0.000045642646,0.00009160793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015194753,0.0002340885,0.00041147938,0.0008657302,0.00047177033,0.00038066015,0.00026346932,0.00032409735,0.0008653945],"category_scores_gemma":[0.00027629512,0.00017906998,0.00014141217,0.00082941767,0.00026449168,0.00018694095,0.00044384485,0.00043802033,0.0003677182],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010379176,0.00014449534,0.16743158,0.00011334551,0.0001311476,0.0012845101,0.00033928826,0.00037900946,0.8155833,0.00030132968,0.0006940196,0.012560116],"study_design_scores_gemma":[0.000066834444,0.00026118752,0.96599513,0.000013296251,0.000053406253,0.0015380393,0.00013281037,0.0012284634,0.028380044,0.0001376586,0.0021727611,0.000020335825],"about_ca_topic_score_codex":0.0029256176,"about_ca_topic_score_gemma":0.00569746,"teacher_disagreement_score":0.0029256176,"about_ca_system_score_codex":0.00024764807,"about_ca_system_score_gemma":0.00020776539,"threshold_uncertainty_score":0.0058172345},"labels":[],"label_agreement":null},{"id":"W2134822887","doi":"10.1088/0004-637x/791/2/106","title":"CARBON SYNTHESIS IN STEADY-STATE HYDROGEN AND HELIUM BURNING ON ACCRETING NEUTRON STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Hydrogen; Helium; Carbon fibers; Accretion (finance); Neutron star; Stars; Neutron; Nucleosynthesis","score_opus":0.009486189650035955,"score_gpt":0.2146894090708082,"score_spread":0.20520321942077224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2134822887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99861133,0.0002617785,0.0004582648,0.000007965961,0.0000019659797,0.0000023225555,0.0000893331,0.000007708479,0.0005592389],"genre_scores_gemma":[0.9992956,0.000120340126,0.00022891928,0.0000057758352,0.0000020179525,0.0000028408178,0.00015994498,0.000006372546,0.0001781829],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998987,0.000020862133,0.000005621165,0.000035933062,0.000020606696,0.000018300902],"domain_scores_gemma":[0.9996791,0.00015378551,0.00006419838,0.000030155474,0.00003453118,0.00003824769],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027551648,0.00022471657,0.0002947921,0.0004835941,0.0002742083,0.00039663608,0.00027881592,0.0002478777,0.00071862945],"category_scores_gemma":[0.00047333247,0.00019335913,0.0001667084,0.00033593428,0.00048045546,0.0003322981,0.00033270926,0.00021206848,0.00017751123],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015104256,0.00010321851,0.1305595,0.00018282374,0.00011166524,0.00033007376,0.00022452133,0.0051326486,0.8475308,0.0011921402,0.00009909865,0.013023137],"study_design_scores_gemma":[0.000054424894,0.0005906344,0.4660584,0.000025227753,0.00006639735,0.00037377104,0.0002075118,0.022772675,0.50659734,0.0021667143,0.0010559334,0.00003099175],"about_ca_topic_score_codex":0.0010794618,"about_ca_topic_score_gemma":0.0011644873,"teacher_disagreement_score":0.0010794618,"about_ca_system_score_codex":0.00039027372,"about_ca_system_score_gemma":0.00013349255,"threshold_uncertainty_score":0.0028316379},"labels":[],"label_agreement":null},{"id":"W2134988917","doi":"10.1088/0004-637x/780/1/75","title":"HerMES: CANDIDATE HIGH-REDSHIFT GALAXIES DISCOVERED WITH<i>HERSCHEL</i>/SPIRE,","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of British Columbia","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Spire (mollusc); Redshift; Luminosity function; Luminosity; Star formation; Population; Luminous infrared galaxy; Flux (metallurgy); Astronomy","score_opus":0.004664669439220515,"score_gpt":0.19054512658699116,"score_spread":0.18588045714777066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2134988917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8175659,0.0011882087,0.03792478,0.00046144848,0.00010428681,0.00023064822,0.08144083,0.012076998,0.049006883],"genre_scores_gemma":[0.82501507,0.0005128781,0.055727817,0.0003073888,0.00014611743,0.00021101937,0.09685395,0.0007036086,0.020522146],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996668,0.00003233079,0.000010983541,0.00011129244,0.000107419204,0.00007121622],"domain_scores_gemma":[0.9993586,0.00006706303,0.00020370197,0.00016429514,0.00006162037,0.00014473686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009052787,0.00044089576,0.00027970437,0.002289821,0.00033285646,0.0006548735,0.00049163186,0.00021575742,0.008196317],"category_scores_gemma":[0.0008157215,0.000255862,0.0003981738,0.0011737787,0.00019887742,0.0004599263,0.0007364524,0.00021755355,0.0036499505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045015206,0.00015283946,0.7153223,0.00023616473,0.00034911043,0.0004887086,0.00057920074,0.003509834,0.034514014,0.00838092,0.08890084,0.1471159],"study_design_scores_gemma":[0.000069293936,0.00009490147,0.88817596,0.000043198597,0.000062519706,0.00038241482,0.00019722487,0.008105955,0.011746321,0.0015449976,0.08953549,0.000041721833],"about_ca_topic_score_codex":0.0059418436,"about_ca_topic_score_gemma":0.019639008,"teacher_disagreement_score":0.008196317,"about_ca_system_score_codex":0.00032456455,"about_ca_system_score_gemma":0.00036107903,"threshold_uncertainty_score":0.027419448},"labels":[],"label_agreement":null},{"id":"W2134996485","doi":"10.1088/0004-637x/813/1/8","title":"COULD JUPITER OR SATURN HAVE EJECTED A FIFTH GIANT PLANET?","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Giant planet; Astronomy; Physics; Planet; Jupiter (rocket family); Gas giant; Solar System; Saturn; Jovian; Astrobiology; Orbit (dynamics); Astrophysics; Planetary system; Exoplanet; Space exploration","score_opus":0.02232953681838833,"score_gpt":0.24067515763219455,"score_spread":0.2183456208138062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2134996485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953236,0.00024037753,0.0012584401,0.00033970736,0.00001646275,0.000005843194,0.000063201594,0.00002120864,0.0027311735],"genre_scores_gemma":[0.9993006,0.000053784763,0.00030756558,0.000039376388,0.0000051531565,0.0000014531042,0.00006767082,0.000003856592,0.00022046115],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998336,0.000024005934,0.0000065967047,0.000046303907,0.000031257787,0.000058261725],"domain_scores_gemma":[0.9988708,0.00042915292,0.00036109638,0.00010979071,0.00004755219,0.0001815549],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007991829,0.00024916552,0.00039987013,0.00050768035,0.0006940306,0.0009881877,0.0005585542,0.0010618253,0.0023480903],"category_scores_gemma":[0.006116676,0.00014879648,0.0004443899,0.00042401187,0.00078562024,0.0013621639,0.0009760183,0.00036623745,0.00017620265],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013433145,0.000057836787,0.83921075,0.00021069279,0.00037286707,0.0038027526,0.0010088941,0.072459824,0.004564535,0.04568215,0.0012549963,0.030031364],"study_design_scores_gemma":[0.00023016515,0.0008954301,0.5566939,0.0003134972,0.00048061687,0.0074684788,0.005962582,0.34230763,0.010956736,0.055000514,0.01954084,0.00014966782],"about_ca_topic_score_codex":0.0049263565,"about_ca_topic_score_gemma":0.0049379827,"teacher_disagreement_score":0.0049263565,"about_ca_system_score_codex":0.0006408197,"about_ca_system_score_gemma":0.00041033168,"threshold_uncertainty_score":0.009795368},"labels":[],"label_agreement":null},{"id":"W2135145559","doi":"10.1088/0004-637x/790/2/137","title":"IMPLICATIONS OF PLASMA BEAM INSTABILITIES FOR THE STATISTICS OF THE<i>FERMI</i>HARD GAMMA-RAY BLAZARS AND THE ORIGIN OF THE EXTRAGALACTIC GAMMA-RAY BACKGROUND","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Blazar; Quasar; Extragalactic background light; Fermi Gamma-ray Space Telescope; Population; Redshift; Luminosity; Accretion (finance)","score_opus":0.01488881096652335,"score_gpt":0.23764535888554178,"score_spread":0.22275654791901844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135145559","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928497,0.00010796908,0.00510558,0.00015593163,0.0000044306003,0.000006931322,0.00011282283,0.00005736601,0.0015993642],"genre_scores_gemma":[0.9994924,0.000029207797,0.00029183118,0.000015991493,0.0000062028726,0.0000024670546,0.000052107476,0.0000052908235,0.0001045105],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998043,0.00004610989,0.0000111608715,0.00006610104,0.000032923603,0.000039427396],"domain_scores_gemma":[0.9984316,0.00055102084,0.0006108609,0.00023557815,0.000069599715,0.000101284764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074774324,0.0003052261,0.00024616806,0.00042999722,0.00034482178,0.0011835677,0.00074521825,0.0005504749,0.0010490402],"category_scores_gemma":[0.003073806,0.0001541232,0.0003636459,0.0002661298,0.000881652,0.0007115653,0.00038776896,0.00041684322,0.00015742367],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045157195,0.00008742467,0.7741056,0.000065759785,0.00014448146,0.0010065738,0.0004983876,0.09616701,0.04548564,0.06676102,0.0008567202,0.0143698165],"study_design_scores_gemma":[0.00006756009,0.00014247089,0.4918553,0.000020416745,0.00006690844,0.0008815157,0.00024070723,0.44898766,0.007790649,0.048460346,0.0014233233,0.00006313986],"about_ca_topic_score_codex":0.00634878,"about_ca_topic_score_gemma":0.003759546,"teacher_disagreement_score":0.00634878,"about_ca_system_score_codex":0.0010413567,"about_ca_system_score_gemma":0.00029646713,"threshold_uncertainty_score":0.012623668},"labels":[],"label_agreement":null},{"id":"W2135148623","doi":"10.1088/0004-637x/739/2/87","title":"<i>Fermi</i>/GAMMA-RAY BURST MONITOR OBSERVATIONS OF SGR J0501+4516 BURSTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Fermi Gamma-ray Space Telescope; Spectral line; Flux (metallurgy); Gamma-ray burst; Black-body radiation; Luminosity; Power law; Light curve; Photon; Cutoff; Magnetar; Spitzer Space Telescope; Neutron star; Astronomy; Telescope; Radiation; Statistics; Galaxy; Optics","score_opus":0.03980252903443328,"score_gpt":0.30578357716040677,"score_spread":0.2659810481259735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135148623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99817204,0.00008274835,0.0002532515,0.00001649106,0.0000028817879,0.00000441254,0.000677571,0.0000552506,0.0007353361],"genre_scores_gemma":[0.99708396,0.000073721356,0.000946198,0.000018393677,0.000008946461,0.0000077682835,0.001582279,0.000011421743,0.00026743262],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999188,0.0000069891266,0.000009488537,0.000022234879,0.000024446965,0.000018023966],"domain_scores_gemma":[0.9997348,0.000026054478,0.0001258148,0.000024515022,0.000034133252,0.000054709617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001936213,0.00027676337,0.00022909482,0.0012942904,0.00019536486,0.00042028003,0.0002989692,0.00021315018,0.00084070704],"category_scores_gemma":[0.00035220906,0.00013420216,0.000347583,0.000646187,0.000103619175,0.00014901783,0.00027807735,0.0001474831,0.00023614483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034539113,0.000071094095,0.9132914,0.00006584711,0.00011999285,0.0004149509,0.00027448888,0.0030519422,0.06068217,0.00023395798,0.0010656988,0.02038319],"study_design_scores_gemma":[0.00000736449,0.000058123533,0.9924482,0.000010369503,0.000029013345,0.00022866295,0.000041495387,0.0031199798,0.003174692,0.000039012953,0.0008342809,0.000008720513],"about_ca_topic_score_codex":0.006125062,"about_ca_topic_score_gemma":0.010613794,"teacher_disagreement_score":0.006125062,"about_ca_system_score_codex":0.00038816157,"about_ca_system_score_gemma":0.00011078376,"threshold_uncertainty_score":0.012178838},"labels":[],"label_agreement":null},{"id":"W2135329435","doi":"10.1086/432252","title":"Magnetospheric Eclipses in the Double Pulsar System PSR J0737−3039","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Pulsar; Physics; Astrophysics; Binary pulsar; Magnetosphere; Millisecond pulsar; Rotation period; Neutron star; Orbital period; Stellar rotation; X-ray pulsar; Astronomy; Eclipse; Magnetic field; Stars","score_opus":0.012828056803135129,"score_gpt":0.30063516417055547,"score_spread":0.2878071073674203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135329435","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877244,0.00005407941,0.00022952785,0.00002131723,0.00000502271,0.0000025833424,0.0000712791,0.000016795699,0.0008269921],"genre_scores_gemma":[0.9995084,0.000030145611,0.00016559717,0.0000064502915,0.0000032288,0.0000042038464,0.00014107065,0.000007797056,0.00013310117],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995553,0.000008900434,0.0000029676676,0.000010705914,0.0000070309325,0.00001480577],"domain_scores_gemma":[0.9999151,0.000019059558,0.000024380752,0.000013991398,0.000008264764,0.000019099805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009226289,0.00021590866,0.0002171921,0.00032046658,0.0003960055,0.0004542715,0.00016429054,0.00027496644,0.00070314837],"category_scores_gemma":[0.0003449492,0.00010406041,0.0002583934,0.00031061523,0.0003616602,0.00018367438,0.0005242135,0.00019762942,0.0001295494],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00145454,0.00026507297,0.47303048,0.000239289,0.00024552562,0.0066772522,0.0014712274,0.28577182,0.14070405,0.040752362,0.0052927933,0.044095647],"study_design_scores_gemma":[0.00024866735,0.00054918183,0.6553716,0.00005159221,0.0001028882,0.0019396741,0.0007946488,0.31248572,0.008325375,0.011025343,0.009025868,0.00007940673],"about_ca_topic_score_codex":0.008131144,"about_ca_topic_score_gemma":0.0069882986,"teacher_disagreement_score":0.008131144,"about_ca_system_score_codex":0.0007592135,"about_ca_system_score_gemma":0.00031898485,"threshold_uncertainty_score":0.01616764},"labels":[],"label_agreement":null},{"id":"W2135332747","doi":"10.1088/0004-637x/788/1/3","title":"CHARACTERIZING THE STRUCTURE OF DIFFUSE EMISSION IN Hi-GAL MAPS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Geography","score_opus":0.006399124897829175,"score_gpt":0.21958724459989445,"score_spread":0.21318811970206528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135332747","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99640465,0.000052577274,0.0026564668,0.0000071121412,9.19435e-7,0.000005043898,0.00012749847,0.000024274288,0.00072147744],"genre_scores_gemma":[0.99826044,0.000030886873,0.0013140731,0.0000031861414,0.0000051167226,0.0000031815325,0.00028074198,0.00000933133,0.00009305252],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999287,0.0000100403595,0.000002670642,0.000021854497,0.000016562171,0.000020189971],"domain_scores_gemma":[0.99962294,0.00010413125,0.000111935566,0.000046590452,0.000058654485,0.00005574286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013352145,0.00012677802,0.00010828887,0.0014399642,0.000099031866,0.0005162868,0.0001769399,0.000112224254,0.000332538],"category_scores_gemma":[0.00075691025,0.00008885746,0.00013813654,0.0007215896,0.00024627277,0.00021268244,0.00029943185,0.00010111133,0.00010026554],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003964918,0.00009256967,0.8029826,0.000098797165,0.00012549042,0.0009845457,0.0012698148,0.022199653,0.10558658,0.004682554,0.0005527019,0.06102809],"study_design_scores_gemma":[0.0000052070895,0.00003458372,0.9801205,0.0000065365057,0.000017555518,0.00021051792,0.00021988236,0.015583063,0.0025298074,0.0007032861,0.0005605524,0.000008516095],"about_ca_topic_score_codex":0.00091846567,"about_ca_topic_score_gemma":0.00088840537,"teacher_disagreement_score":0.0014399642,"about_ca_system_score_codex":0.00012325252,"about_ca_system_score_gemma":0.00006588142,"threshold_uncertainty_score":0.0018262267},"labels":[],"label_agreement":null},{"id":"W2135497511","doi":"10.1086/589937","title":"Improved Cosmological Constraints from New, Old, and Combined Supernova Data Sets","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1559,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Nuclear Physics; Science and Technology Facilities Council; Office of Science; Fundação para a Ciência e a Tecnologia; U.S. Department of Energy; University of Arizona; Deutsche Forschungsgemeinschaft; Yale University","keywords":"Physics; Cosmic microwave background; Dark energy; Supernova; Redshift; Astrophysics; Hubble's law; Cosmological constant; Equation of state; Cosmology; Theoretical physics; Galaxy","score_opus":0.03188586802557097,"score_gpt":0.24808694507484685,"score_spread":0.21620107704927588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135497511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.85600775,0.002541933,0.09914991,0.0004073243,0.00011337845,0.000092967406,0.031783383,0.0008663884,0.009036997],"genre_scores_gemma":[0.76235276,0.0014092043,0.1453325,0.00020990855,0.00046744273,0.00018998647,0.08751582,0.00052361784,0.001998673],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9948762,0.0013335943,0.0006500418,0.0010112781,0.0018726249,0.0002561881],"domain_scores_gemma":[0.9740918,0.009581743,0.003063346,0.007746238,0.004017335,0.0014994858],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.009015541,0.0008747044,0.0016234106,0.00572029,0.00083971437,0.0034170893,0.0015678625,0.00036926862,0.0024715848],"category_scores_gemma":[0.023002306,0.0009662409,0.0008854391,0.0039362037,0.00054009754,0.0027951314,0.0042436137,0.0012303981,0.0006355116],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011003768,0.0004487602,0.7237798,0.00058390433,0.0023663943,0.00034728702,0.0007692242,0.033402827,0.017193377,0.016946288,0.011887608,0.19117422],"study_design_scores_gemma":[0.00023961156,0.00019076173,0.83637017,0.00021743434,0.00094504724,0.000583666,0.00035616526,0.08587882,0.009957073,0.01658201,0.048405986,0.00027332682],"about_ca_topic_score_codex":0.0063917814,"about_ca_topic_score_gemma":0.017806515,"teacher_disagreement_score":0.009015541,"about_ca_system_score_codex":0.0006375818,"about_ca_system_score_gemma":0.00088522315,"threshold_uncertainty_score":0.047679305},"labels":[],"label_agreement":null},{"id":"W2135959397","doi":"10.1086/588212","title":"An Infrared Survey of Brightest Cluster Galaxies. II. Why are Some Brightest Cluster Galaxies Forming Stars?","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":272,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"University of Rochester; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Star formation; Luminosity; Galaxy; Cluster (spacecraft); Infrared; Galaxy cluster; Spitzer Space Telescope; Intracluster medium; Luminous infrared galaxy","score_opus":0.013875424854418252,"score_gpt":0.2202751179910843,"score_spread":0.20639969313666603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2135959397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98959863,0.0027589551,0.00030390025,0.00045858324,0.00003060433,0.000022314507,0.0025673078,0.000051766932,0.004207912],"genre_scores_gemma":[0.994909,0.0007341425,0.0005765069,0.00019734469,0.000047993057,0.0000119822325,0.0020969792,0.000007833479,0.0014181561],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980694,0.000020911968,0.000011355737,0.000047119287,0.00004809548,0.00006562266],"domain_scores_gemma":[0.9992618,0.000056183224,0.00018562748,0.00006861285,0.00022997125,0.00019776683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005203129,0.00018870675,0.00022505705,0.0023588224,0.0004354066,0.00058891793,0.00028684587,0.00026274336,0.0017456174],"category_scores_gemma":[0.0005035213,0.00013284772,0.0002211244,0.0014756373,0.00022689966,0.00034421615,0.00029437224,0.00024348717,0.0007948073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005404436,0.0000244805,0.98099524,0.000042352276,0.000051124174,0.00006774966,0.0002389457,0.000034128254,0.004071851,0.00015367172,0.0018196191,0.012446774],"study_design_scores_gemma":[0.0000015265559,0.000009444859,0.9990085,0.0000042189736,0.00000986663,0.00004175661,0.000092936476,0.00001438146,0.000106844935,0.00001503975,0.0006944545,0.000001163765],"about_ca_topic_score_codex":0.016305545,"about_ca_topic_score_gemma":0.029782705,"teacher_disagreement_score":0.016305545,"about_ca_system_score_codex":0.00046918375,"about_ca_system_score_gemma":0.00024176859,"threshold_uncertainty_score":0.03242123},"labels":[],"label_agreement":null},{"id":"W2136015545","doi":"10.1088/0004-637x/703/1/169","title":"SIMULTANEOUS MULTIWAVELENGTH OBSERVATIONS OF MARKARIAN 421 DURING OUTBURST","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Max-Planck-Gesellschaft; Bundesministerium für Bildung und Forschung; National Science Foundation; Science Foundation Ireland; National Aeronautics and Space Administration; Helmholtz-Gemeinschaft; U.S. Department of Energy; Smithsonian Institution","keywords":"Blazar; Physics; Astrophysics; Telescope; MAGIC (telescope); Gamma ray; Astronomy; X-ray telescope; Spectral energy distribution; Wavelength; Observatory; Galaxy; Optics","score_opus":0.010153075208659924,"score_gpt":0.2181955447812944,"score_spread":0.20804246957263448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136015545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988445,0.0000690686,0.0001497031,0.000015398446,0.0000026530586,0.0000033457236,0.00014535857,0.000030388805,0.0007395337],"genre_scores_gemma":[0.9980794,0.000071803785,0.0005275933,0.000022327235,0.000009233387,0.0000055175938,0.00075577927,0.000021171827,0.0005071582],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984694,0.000011934225,0.000005277982,0.000049498834,0.00004112867,0.000045197125],"domain_scores_gemma":[0.99959177,0.00003155356,0.00015802048,0.00005054999,0.000052317966,0.0001158037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002278086,0.00027788867,0.0005294235,0.000683262,0.00057616207,0.0005439993,0.0003246828,0.00031712672,0.000474571],"category_scores_gemma":[0.00036206815,0.00028900296,0.00026625593,0.0005159414,0.00015862849,0.00023518603,0.0007098453,0.00043049367,0.00020730493],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012432153,0.0002564495,0.78189427,0.00011382266,0.00035116667,0.0014826094,0.0023937735,0.0025467752,0.17913869,0.00034192402,0.001190127,0.02904715],"study_design_scores_gemma":[0.00001018627,0.00007058553,0.99520975,0.0000034450788,0.000028199673,0.00015543996,0.00015997441,0.00039553022,0.0028591326,0.000030650062,0.0010689241,0.000008243887],"about_ca_topic_score_codex":0.0050635114,"about_ca_topic_score_gemma":0.01643039,"teacher_disagreement_score":0.0050635114,"about_ca_system_score_codex":0.00030589438,"about_ca_system_score_gemma":0.00016995924,"threshold_uncertainty_score":0.010068059},"labels":[],"label_agreement":null},{"id":"W2136195529","doi":"10.1088/0004-637x/779/2/91","title":"MOA-2010-BLG-328Lb: A SUB-NEPTUNE ORBITING VERY LATE M DWARF?","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Science and Technology Facilities Council","keywords":"Physics; Gravitational microlensing; Parallax; Neptune; Proper motion; Planet; Astronomy; Astrophysics; Planetary system; Solar System; Stars","score_opus":0.010779832386955644,"score_gpt":0.20728385805834998,"score_spread":0.19650402567139433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136195529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89069486,0.00064022926,0.001159087,0.003176712,0.0005817452,0.00006026563,0.0034403587,0.0006779593,0.099568695],"genre_scores_gemma":[0.9542164,0.00014151116,0.0016840413,0.0008629834,0.000076211014,0.000013053807,0.0044167433,0.000096092095,0.038492948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999944,0.0000045802226,0.0000013577127,0.000016266693,0.000011644922,0.0000221489],"domain_scores_gemma":[0.99982256,0.0000070673864,0.000014202666,0.000012829631,0.000029581228,0.00011378815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001374858,0.00011336662,0.000151668,0.00031267814,0.0014296678,0.00055257266,0.0002542514,0.0004909872,0.004576939],"category_scores_gemma":[0.00024235457,0.000052253366,0.00008836298,0.00033951632,0.0003371734,0.00036634918,0.00057547825,0.0004417051,0.002246823],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0029488748,0.00090113055,0.4052303,0.00023553288,0.00009205304,0.020972004,0.0065786624,0.0011588979,0.12325843,0.02440935,0.16266233,0.25155234],"study_design_scores_gemma":[0.00011015707,0.0006124838,0.42355034,0.000075587566,0.000031527976,0.008378007,0.0047508003,0.002478299,0.005996286,0.0038987629,0.55006814,0.00004961424],"about_ca_topic_score_codex":0.020072984,"about_ca_topic_score_gemma":0.04556486,"teacher_disagreement_score":0.020072984,"about_ca_system_score_codex":0.0006710306,"about_ca_system_score_gemma":0.0005371998,"threshold_uncertainty_score":0.039912343},"labels":[],"label_agreement":null},{"id":"W2136196166","doi":"10.1088/0004-637x/691/1/560","title":"DO SUBMILLIMETER GALAXIES REALLY TRACE THE MOST MASSIVE DARK-MATTER HALOS? DISCOVERY OF A HIGH-<i>z</i>CLUSTER IN A HIGHLY ACTIVE PHASE OF EVOLUTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Redshift; Stellar mass; Galaxy cluster; Galaxy formation and evolution; Cluster (spacecraft); Active galactic nucleus; Billion years; Phase (matter)","score_opus":0.005885333440887444,"score_gpt":0.2217110118867865,"score_spread":0.21582567844589906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136196166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99930453,0.000036113444,0.00010815932,0.000041538744,0.0000012887169,0.0000012868439,0.00013520186,0.000010022301,0.00036175808],"genre_scores_gemma":[0.9995003,0.000023246264,0.00015888788,0.000021755779,0.0000040880664,0.0000012320234,0.000197445,0.0000042269526,0.00008879858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991083,0.000006340589,0.000003189042,0.000027076681,0.000017259112,0.00003521584],"domain_scores_gemma":[0.9993975,0.00007080789,0.00025410345,0.0000593975,0.000037688653,0.00018047662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023477335,0.0001404311,0.0002911765,0.00077018235,0.00041869452,0.0007851162,0.00030953006,0.00033829405,0.0011255259],"category_scores_gemma":[0.000662074,0.00021328739,0.0001482453,0.0008223088,0.00040241578,0.00043970667,0.0005293473,0.00031843522,0.00023636963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000799934,0.000019746916,0.9863522,0.000009672027,0.000022585198,0.00010066908,0.00030494205,0.00012561861,0.0096190125,0.0002366185,0.0001747913,0.002954143],"study_design_scores_gemma":[0.0000013410398,0.000010291374,0.99911433,0.0000016936107,0.0000041110357,0.000045947785,0.00009723149,0.0001855001,0.00031293402,0.00006421677,0.00016020813,0.0000022753495],"about_ca_topic_score_codex":0.005080517,"about_ca_topic_score_gemma":0.010466192,"teacher_disagreement_score":0.005080517,"about_ca_system_score_codex":0.00029803658,"about_ca_system_score_gemma":0.000105587125,"threshold_uncertainty_score":0.010101914},"labels":[],"label_agreement":null},{"id":"W2136216244","doi":"10.1088/0004-637x/734/2/117","title":"WARM SATURNS: ON THE NATURE OF RINGS AROUND EXTRASOLAR PLANETS THAT RESIDE INSIDE THE ICE LINE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Exoplanet; Physics; Planet; RADIUS; Astronomy; Astrophysics; Planetary system; Solar System; Transit (satellite); Earth radius; Astrobiology","score_opus":0.02444275235889317,"score_gpt":0.22781409451966914,"score_spread":0.20337134216077596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136216244","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99416465,0.0012332464,0.00023868539,0.00015887852,0.000010619499,0.0000043167524,0.000108515334,0.0000057927214,0.0040751724],"genre_scores_gemma":[0.9990338,0.00028056558,0.00010486231,0.00002943802,0.000031846943,0.0000013480478,0.00008592404,0.000004960546,0.0004272616],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999187,0.0000096039275,0.000002516834,0.000025204285,0.000010932493,0.00003302442],"domain_scores_gemma":[0.99955076,0.00008052975,0.00016937204,0.00004448356,0.00006250925,0.0000923095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027269512,0.000108620836,0.00017470335,0.00045255283,0.00052222435,0.0005768382,0.00028524967,0.0003100729,0.0010255553],"category_scores_gemma":[0.000659774,0.000091779046,0.00014740857,0.00018462095,0.0004770424,0.0007420753,0.0006238751,0.00022170052,0.00022125285],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006207639,0.00005017919,0.872708,0.00014156668,0.0001314055,0.0009918483,0.0029352105,0.0009414806,0.09818519,0.0028110207,0.00077884406,0.019704474],"study_design_scores_gemma":[0.0000045277934,0.000057491143,0.9942973,0.000014806741,0.00001793397,0.00037920533,0.000705079,0.00044106544,0.0017775244,0.0003293726,0.0019685826,0.000007061352],"about_ca_topic_score_codex":0.0034310566,"about_ca_topic_score_gemma":0.0075494163,"teacher_disagreement_score":0.0034310566,"about_ca_system_score_codex":0.0004160217,"about_ca_system_score_gemma":0.00008119612,"threshold_uncertainty_score":0.006822169},"labels":[],"label_agreement":null},{"id":"W2136273233","doi":"10.1086/320635","title":"Radio Pulsars in the Magellanic Clouds","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Millisecond pulsar; Astrophysics; Large Magellanic Cloud; Astronomy; Small Magellanic Cloud; Radio telescope; Stars","score_opus":0.01404857102429699,"score_gpt":0.31174132420011685,"score_spread":0.2976927531758199,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136273233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99696726,0.0015346373,0.00027827252,0.000054916687,0.0000111898635,0.0000042138804,0.000160339,0.000017696133,0.00097149995],"genre_scores_gemma":[0.99763334,0.00088969903,0.00042874477,0.00003561114,0.00004354356,0.000004118077,0.00048623147,0.0000038232865,0.00047493418],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976546,0.00001890431,0.0000082500455,0.00004885709,0.00005834294,0.0001001908],"domain_scores_gemma":[0.99892884,0.00019510716,0.00045116106,0.00008338787,0.00013788305,0.00020354176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029935222,0.00023083661,0.00019887702,0.0016332632,0.0004998835,0.00051704,0.0002654499,0.0002616347,0.000902349],"category_scores_gemma":[0.0011071307,0.000119442775,0.00013332184,0.0015930731,0.00028922482,0.000430624,0.0007611615,0.00020266806,0.00025901076],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001772257,0.000057377463,0.9277771,0.00006255851,0.00006125305,0.0005052921,0.00048403468,0.0005259601,0.025132509,0.0005990021,0.00062769314,0.043990094],"study_design_scores_gemma":[0.000011812772,0.00013097118,0.9901342,0.00001538161,0.000045128905,0.0009532274,0.00016663264,0.0002979394,0.0028419914,0.0004041756,0.004991069,0.0000074896598],"about_ca_topic_score_codex":0.0022931984,"about_ca_topic_score_gemma":0.0031242617,"teacher_disagreement_score":0.0022931984,"about_ca_system_score_codex":0.00023613873,"about_ca_system_score_gemma":0.000158881,"threshold_uncertainty_score":0.004559636},"labels":[],"label_agreement":null},{"id":"W2136304890","doi":"10.1088/0004-637x/811/2/126","title":"BICEP2/KECK ARRAY V: MEASUREMENTS OF<i>B</i>-MODE POLARIZATION AT DEGREE ANGULAR SCALES AND 150 GHz BY THE KECK ARRAY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; University of British Columbia; University of Toronto","funders":"SLAC National Accelerator Laboratory; Harvard University; U.S. Department of Energy; Gordon and Betty Moore Foundation; W. M. Keck Foundation; Office of Science; California Institute of Technology; National Aeronautics and Space Administration; Advanced Research Projects Agency; National Science Foundation","keywords":"Cosmic microwave background; Polarization (electrochemistry); Calibration; Cosmic background radiation; Jackknife resampling; Microwave; Range (aeronautics); Cosmic infrared background","score_opus":0.03253936189580514,"score_gpt":0.24450785962627836,"score_spread":0.21196849773047322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136304890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93705887,0.0004872106,0.018277148,0.00025244715,0.00007418727,0.00012238833,0.017914414,0.0011058664,0.024707522],"genre_scores_gemma":[0.9512846,0.00014237282,0.02601552,0.00021968725,0.000057669546,0.00019955727,0.018629739,0.00043854353,0.0030122425],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99887735,0.00018026918,0.00004101624,0.0003306478,0.00033893177,0.00023188912],"domain_scores_gemma":[0.9986425,0.00014826976,0.00019465691,0.0004117713,0.00036474442,0.00023800513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011591811,0.00058127585,0.0004552944,0.0013341842,0.0006706633,0.0010832972,0.0007669751,0.00059850904,0.0029678845],"category_scores_gemma":[0.0012832613,0.00055654626,0.0004866804,0.0018479368,0.00036851288,0.0010483204,0.0014300238,0.0008398024,0.0010541797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0044716108,0.00081966555,0.48141912,0.00042554055,0.0009401115,0.0008778306,0.0009769462,0.015853755,0.38369024,0.0047062477,0.024872154,0.08094677],"study_design_scores_gemma":[0.00016689168,0.0002369608,0.89552814,0.000037726062,0.00014155918,0.000606109,0.00012524141,0.010691747,0.07588529,0.0005442764,0.01592958,0.00010654625],"about_ca_topic_score_codex":0.00677851,"about_ca_topic_score_gemma":0.011745675,"teacher_disagreement_score":0.00677851,"about_ca_system_score_codex":0.00047989518,"about_ca_system_score_gemma":0.00045162346,"threshold_uncertainty_score":0.0134781},"labels":[],"label_agreement":null},{"id":"W2136386395","doi":"10.1086/340018","title":"The Central Binary and Surrounding Nebula of the Symbiotic Star V1016 Cygni","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Nebula; Astrophysics; Planetary nebula; Symbiotic star; Astronomy; Stars; Emission nebula; Position angle; Space Telescope Imaging Spectrograph; Emission spectrum; Bipolar outflow; Spectrograph; Reflection nebula; Telescope; Doubly ionized oxygen; Hubble space telescope; Spectral line; Star formation; Galaxy","score_opus":0.011226431928412208,"score_gpt":0.2021313719968159,"score_spread":0.1909049400684037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136386395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960443,0.00024601643,0.000115896946,0.000023929917,0.0000042427027,0.000004053372,0.00025548018,0.000015604466,0.0032905021],"genre_scores_gemma":[0.9980387,0.00008805501,0.0003354136,0.000011873749,0.0000046783075,0.0000020320936,0.00061262783,0.000006076473,0.0009006815],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997246,0.0000013395394,7.8879145e-7,0.00000764844,0.0000071411005,0.000010605571],"domain_scores_gemma":[0.9999429,0.0000042378997,0.0000130635635,0.0000046669384,0.0000045150514,0.000030555275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004723554,0.00015462073,0.00017400213,0.0004505004,0.00037279565,0.00034563045,0.00013152212,0.00018623819,0.0018161028],"category_scores_gemma":[0.00014825788,0.000080726415,0.0000603671,0.00035289887,0.00017931925,0.00016320369,0.00047347462,0.00012265774,0.00032090838],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011360516,0.0002191123,0.21048936,0.00023146384,0.000045350214,0.007933196,0.0009806167,0.003212869,0.73240536,0.0031416337,0.0021470706,0.03805792],"study_design_scores_gemma":[0.000027123544,0.00012838241,0.97011524,0.000018506338,0.000015426847,0.0037686361,0.00021623156,0.0040946584,0.016312359,0.0006359043,0.0046571274,0.000010403722],"about_ca_topic_score_codex":0.0057963296,"about_ca_topic_score_gemma":0.004948697,"teacher_disagreement_score":0.0057963296,"about_ca_system_score_codex":0.0002884326,"about_ca_system_score_gemma":0.00013173952,"threshold_uncertainty_score":0.011525214},"labels":[],"label_agreement":null},{"id":"W2136444955","doi":"10.1088/0004-637x/692/2/1411","title":"BLUE STRAGGLERS AFTER THE MAIN SEQUENCE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Blue straggler; Sequence (biology); Asymptotic giant branch; Horizontal branch; Red-giant branch; Main sequence; Stars","score_opus":0.01213184676832895,"score_gpt":0.23054026905231417,"score_spread":0.21840842228398522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136444955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992532,0.00015634055,0.00011973815,0.000008725907,0.000002121971,0.0000018267883,0.00004751789,0.0000048468382,0.00040559136],"genre_scores_gemma":[0.99708813,0.00011996179,0.00010303796,0.0000144076575,0.0000041441376,0.000002669692,0.00025005618,0.000010278499,0.00240734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999293,0.0000071350673,0.000001519497,0.000019313393,0.000013470865,0.000029215746],"domain_scores_gemma":[0.9994011,0.00009065487,0.00018938744,0.000031843738,0.00007231856,0.00021464852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023986587,0.00024349435,0.00022853172,0.00049962243,0.00046939985,0.0004926031,0.00031743103,0.00028304826,0.0024570418],"category_scores_gemma":[0.0007848282,0.00013461537,0.00016355592,0.00036937228,0.00024251455,0.00025901894,0.0004696182,0.00032786676,0.0008534335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009817963,0.00015198725,0.9427525,0.000034631976,0.000063424515,0.0013105014,0.001172876,0.0009282102,0.037715953,0.0023175566,0.00037477232,0.012195724],"study_design_scores_gemma":[0.000014920367,0.000537477,0.9882273,0.0000137654615,0.000025997448,0.0011979247,0.00065086107,0.0015989948,0.0044656834,0.0007643805,0.0024911645,0.000011612437],"about_ca_topic_score_codex":0.004414558,"about_ca_topic_score_gemma":0.0067612957,"teacher_disagreement_score":0.004414558,"about_ca_system_score_codex":0.00036188628,"about_ca_system_score_gemma":0.00023264777,"threshold_uncertainty_score":0.008777738},"labels":[],"label_agreement":null},{"id":"W2136555805","doi":"10.1086/432594","title":"A Bayesian Analysis of Extrasolar Planet Data for HD 73526","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":230,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Exoplanet; Orbit (dynamics); Markov chain Monte Carlo; Radial velocity; Eccentricity (behavior); Bayesian probability; Planet; Astrophysics; Monte Carlo method; Orbital period; Stars; Astronomy; Algorithm; Statistics; Mathematics","score_opus":0.020360634973623594,"score_gpt":0.2596838294755473,"score_spread":0.23932319450192371,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136555805","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1614756,0.0001379472,0.8332108,0.00020276246,0.000019321793,0.00009954828,0.0013110538,0.0018036828,0.0017392476],"genre_scores_gemma":[0.4783619,0.00012933167,0.51473993,0.00005725785,0.000043837146,0.00016384487,0.004429052,0.00045275988,0.0016220759],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994025,0.0002448675,0.000033026197,0.00011286114,0.00016568467,0.000040986222],"domain_scores_gemma":[0.998095,0.00111992,0.00024169851,0.00017131948,0.0002862491,0.000085910375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022918165,0.0005550152,0.0005464853,0.001785841,0.00061800884,0.0008174902,0.00084216066,0.00053497753,0.002057448],"category_scores_gemma":[0.0071991095,0.00040655548,0.0008706897,0.000839738,0.00027421795,0.00073542143,0.0011009884,0.0009100951,0.00058069796],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042364365,0.00029216698,0.047232863,0.00016430089,0.00034931407,0.0003574078,0.00050751085,0.41076818,0.017928813,0.021559233,0.0064064404,0.49401012],"study_design_scores_gemma":[0.00002983073,0.00003046557,0.014885043,0.0000118686285,0.000022437096,0.000065296765,0.000031205385,0.97198063,0.0014386149,0.010173716,0.0012981077,0.00003271332],"about_ca_topic_score_codex":0.013366878,"about_ca_topic_score_gemma":0.019694803,"teacher_disagreement_score":0.013366878,"about_ca_system_score_codex":0.00077236525,"about_ca_system_score_gemma":0.0012769147,"threshold_uncertainty_score":0.026578128},"labels":[],"label_agreement":null},{"id":"W2136555899","doi":"10.1088/0004-637x/748/2/82","title":"MILLIHERTZ QUASI-PERIODIC OSCILLATIONS AND THERMONUCLEAR BURSTS FROM TERZAN 5: A SHOWCASE OF BURNING REGIMES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Physics; Astrophysics; Thermonuclear fusion; Neutron star; Accretion (finance); Eddington luminosity; Luminosity; Globular cluster; Helium; Millisecond pulsar; Context (archaeology); Nuclear physics; Plasma; Galaxy; Atomic physics","score_opus":0.0149220578174627,"score_gpt":0.2313048762397219,"score_spread":0.2163828184222592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136555899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993538,0.00010310077,0.000102072634,0.00000415182,9.905898e-7,0.0000021242988,0.00008210899,0.0000037257225,0.00034801074],"genre_scores_gemma":[0.99877924,0.00013976124,0.00029595752,0.000006567413,0.000005740805,0.00000336055,0.00047927655,0.000004854589,0.00028532807],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999596,0.0000029098742,0.000002610888,0.000013316258,0.000011135492,0.000010442307],"domain_scores_gemma":[0.9998703,0.000018756638,0.000061685925,0.000014730964,0.0000105234885,0.000023940924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000084514504,0.00015331045,0.00014714708,0.000745436,0.00019955667,0.0002602348,0.00018363235,0.00015929072,0.00034400864],"category_scores_gemma":[0.00018943868,0.00008558252,0.00015254576,0.0005476698,0.00019703146,0.00015572587,0.00038822857,0.00013259576,0.000076737284],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069249055,0.00006997977,0.76347977,0.00018515586,0.00014886577,0.0027040187,0.0018455393,0.0034298033,0.1978102,0.0006767229,0.00022882261,0.02872858],"study_design_scores_gemma":[0.0000051818947,0.00006331446,0.9933956,0.0000068570102,0.000019163204,0.00052596896,0.00018847252,0.0013762978,0.0034959936,0.00012431579,0.0007913459,0.0000074589398],"about_ca_topic_score_codex":0.0020611922,"about_ca_topic_score_gemma":0.003183532,"teacher_disagreement_score":0.0020611922,"about_ca_system_score_codex":0.00020768141,"about_ca_system_score_gemma":0.00007774408,"threshold_uncertainty_score":0.004098356},"labels":[],"label_agreement":null},{"id":"W2136580797","doi":"10.1088/0004-637x/740/1/16","title":"OBSERVATION OF ANISOTROPY IN THE ARRIVAL DIRECTIONS OF GALACTIC COSMIC RAYS AT MULTIPLE ANGULAR SCALES WITH IceCube","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Physics; Right ascension; Cosmic ray; Declination; Astrophysics; Anisotropy; Sky; Angular resolution (graph drawing); Neutrino; Muon; Flux (metallurgy); Astronomy; Isotropy; Intensity (physics); Nuclear physics; Optics","score_opus":0.01884044115747753,"score_gpt":0.21387734680609546,"score_spread":0.19503690564861792,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136580797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9498312,0.00042021365,0.006395891,0.00028187927,0.00005355369,0.00006081145,0.016677894,0.00069109484,0.025587572],"genre_scores_gemma":[0.97112817,0.00034354825,0.009925349,0.00008510506,0.0000572623,0.000048008256,0.017036734,0.00013333528,0.0012424375],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995994,0.00006734822,0.000014490689,0.00009085861,0.00015895546,0.00006895811],"domain_scores_gemma":[0.9989736,0.00018716985,0.00027450806,0.0002040996,0.00025575692,0.0001047952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058982294,0.00030311613,0.00035548335,0.0012277862,0.00033414413,0.00063025847,0.00022724693,0.00018004465,0.0011426378],"category_scores_gemma":[0.001249807,0.00024655234,0.00023633335,0.0020553607,0.00033866352,0.00035581493,0.0005608684,0.00055490446,0.00031491223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016307995,0.00019463418,0.8195145,0.0001726323,0.00046542357,0.0006310106,0.00076835335,0.012346302,0.08997018,0.003915793,0.01731869,0.05307174],"study_design_scores_gemma":[0.00003845936,0.000052431078,0.96031994,0.00002734143,0.000051738607,0.0003566243,0.00011469236,0.010236584,0.015034118,0.0007247449,0.013012569,0.00003068719],"about_ca_topic_score_codex":0.008866317,"about_ca_topic_score_gemma":0.022281723,"teacher_disagreement_score":0.008866317,"about_ca_system_score_codex":0.0005752704,"about_ca_system_score_gemma":0.00031389252,"threshold_uncertainty_score":0.017629385},"labels":[],"label_agreement":null},{"id":"W2136645202","doi":"10.1086/588802","title":"<i>FUSE</i>Observations of the Loop I/Local Bubble Interaction Region","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Line-of-sight; Astrophysics; Local Bubble; Photon; Superbubble; Line (geometry); Loop (graph theory); Emission spectrum; Bubble; Ultraviolet; Intensity (physics); Interstellar medium; Astronomy; Optics; Spectral line; Galaxy; Geometry","score_opus":0.028635160324486177,"score_gpt":0.2131456276674589,"score_spread":0.18451046734297272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136645202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99034005,0.00022266695,0.0017013304,0.000044361204,0.000006978521,0.0000105288855,0.0015257073,0.0002762114,0.0058721965],"genre_scores_gemma":[0.99577063,0.000052706728,0.002138497,0.000032049444,0.000008641388,0.000005862142,0.0014781326,0.000022648139,0.0004907972],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999163,0.0000033118054,0.0000020914922,0.000022558732,0.00002437834,0.00003122861],"domain_scores_gemma":[0.99979705,0.00001814667,0.000065061125,0.000022965103,0.000028246295,0.00006850428],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009998054,0.0001615324,0.00016663069,0.0006748877,0.0004058451,0.0003006582,0.00024287043,0.00026267173,0.0012566084],"category_scores_gemma":[0.00022545588,0.0001369649,0.00024189081,0.00035802153,0.00015834771,0.00030348482,0.00046170576,0.00029910918,0.00021280091],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008159022,0.00012214402,0.32840717,0.00009761415,0.00019207469,0.000904328,0.0012782584,0.004349194,0.6327432,0.0017941009,0.0036089611,0.025687022],"study_design_scores_gemma":[0.000025070252,0.00014494675,0.9490552,0.000017526292,0.000091695656,0.000599134,0.0001902453,0.0057119033,0.03767053,0.00037440236,0.006085264,0.000034092292],"about_ca_topic_score_codex":0.015376947,"about_ca_topic_score_gemma":0.022738568,"teacher_disagreement_score":0.015376947,"about_ca_system_score_codex":0.00054448616,"about_ca_system_score_gemma":0.00013166002,"threshold_uncertainty_score":0.030574918},"labels":[],"label_agreement":null},{"id":"W2136664099","doi":"10.1088/0004-637x/694/1/396","title":"THE ROLE OF COLD FLOWS IN THE ASSEMBLY OF GALAXY DISKS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":348,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Accretion (finance); Galaxy; Cooling flow; Virial mass; Virial theorem; Halo; Star formation; Galaxy formation and evolution; RADIUS; Redshift","score_opus":0.005410198747819439,"score_gpt":0.21318323288677696,"score_spread":0.2077730341389575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136664099","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9894852,0.0002960803,0.004939632,0.00035941385,0.00003950159,0.000017356671,0.00014825694,0.000114270566,0.00460028],"genre_scores_gemma":[0.9978841,0.00012411168,0.0012891152,0.000047187295,0.000019436844,0.000008486244,0.00005980572,0.000027993941,0.0005396974],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985456,0.000046816847,0.0000053202707,0.000025406634,0.000017715136,0.00005000943],"domain_scores_gemma":[0.9992193,0.00025222654,0.00018354208,0.00006913379,0.00006107952,0.00021465265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056574924,0.00056484615,0.0004195525,0.00062710105,0.0010414078,0.0017423185,0.0009092128,0.0010640221,0.0013137739],"category_scores_gemma":[0.0034562421,0.00054276845,0.00042444395,0.0003715014,0.0014119605,0.0014905347,0.0011057573,0.00059675664,0.00018596617],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023279307,0.0001269292,0.032558247,0.0000428405,0.00007703793,0.0004103397,0.00031500898,0.94041234,0.0054190396,0.016142461,0.00077395304,0.0034889139],"study_design_scores_gemma":[0.000100513505,0.000052552747,0.00878767,0.000007672746,0.000026880227,0.000045039873,0.0000817742,0.9844072,0.00062208605,0.005283802,0.000559321,0.000025527692],"about_ca_topic_score_codex":0.028075999,"about_ca_topic_score_gemma":0.01438646,"teacher_disagreement_score":0.028075999,"about_ca_system_score_codex":0.0019663197,"about_ca_system_score_gemma":0.00085592637,"threshold_uncertainty_score":0.055825174},"labels":[],"label_agreement":null},{"id":"W2136795586","doi":"10.1086/309346","title":"Laboratory Studies of Ion/Molecule Reactions of Fullerenes: Chemical Derivatization of Fullerenes within Dense Interstellar Clouds and Circumstellar Shells","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Fullerene Chemistry and Applications","field":"Chemistry","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Fullerene; Astrochemistry; Ion; Fullerene chemistry; Molecule; Ionization; Chemical physics; Physics; Interstellar medium; Photochemistry; Astrophysics; Chemistry; Galaxy","score_opus":0.013506773195662635,"score_gpt":0.24321796370575807,"score_spread":0.22971119051009545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136795586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99588215,0.00054224196,0.0022921138,0.000055267235,0.000008991369,0.000032064898,0.00015523794,0.000044782046,0.0009871359],"genre_scores_gemma":[0.9946419,0.00061422645,0.0035849437,0.00004811608,0.000017160639,0.00002154455,0.00040541225,0.000011209297,0.00065546297],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99986076,0.000015529926,0.000006202331,0.000040701198,0.000046388872,0.000030420537],"domain_scores_gemma":[0.99983704,0.000046597586,0.000052126783,0.000017330836,0.000026525171,0.00002028767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028926262,0.00035175218,0.00020685852,0.0003105658,0.0007169176,0.00028646737,0.00042077372,0.00042915097,0.0011000612],"category_scores_gemma":[0.00023692448,0.00012505912,0.00027637917,0.00023947419,0.0006937572,0.0004734198,0.0003448918,0.00052763935,0.00023176904],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013135897,0.00005836462,0.0029514453,0.00006215181,0.000015317482,0.00011557595,0.0001220872,0.00025482412,0.9940684,0.00026003824,0.000058276746,0.0019023624],"study_design_scores_gemma":[0.000022390375,0.0006122429,0.007979595,0.0000042253137,0.000016970156,0.00035158236,0.00007591162,0.0005842082,0.98895246,0.000087623,0.0013002761,0.000012488497],"about_ca_topic_score_codex":0.0019482056,"about_ca_topic_score_gemma":0.0014510723,"teacher_disagreement_score":0.0019482056,"about_ca_system_score_codex":0.00043396518,"about_ca_system_score_gemma":0.00021978839,"threshold_uncertainty_score":0.0038737059},"labels":[],"label_agreement":null},{"id":"W2136940746","doi":"10.1088/0004-637x/722/2/1148","title":"THE ATACAMA COSMOLOGY TELESCOPE: A MEASUREMENT OF THE 600 &lt; ℓ &lt; 8000 COSMIC MICROWAVE BACKGROUND POWER SPECTRUM AT 148 GHz","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Cosmic microwave background; Physics; CMB cold spot; Astrophysics; Galaxy; Spectral density; Cosmic background radiation; Astronomy; Cosmology; Amplitude; Cosmic infrared background; Optics; Anisotropy","score_opus":0.008798240196934816,"score_gpt":0.22797850293090544,"score_spread":0.21918026273397062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136940746","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8651588,0.0009554016,0.009815942,0.0013296626,0.0002379841,0.00015612306,0.021067064,0.0010847439,0.100194216],"genre_scores_gemma":[0.9668578,0.00047761857,0.013236517,0.00037961558,0.00019586159,0.000082923914,0.008353168,0.00017358169,0.0102430545],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995608,0.000052538886,0.000011705482,0.00009872843,0.00023488388,0.0000413534],"domain_scores_gemma":[0.9993425,0.00006120117,0.00014053633,0.00010431849,0.00019813149,0.00015332553],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005043761,0.00019773761,0.00016679411,0.0014768161,0.0006521608,0.0008455269,0.00042748387,0.00055951945,0.0038906238],"category_scores_gemma":[0.0011701827,0.00018245618,0.00013617377,0.0020866264,0.00034145484,0.0006053422,0.0006565339,0.000645338,0.0011581001],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064563786,0.0003570267,0.6428146,0.0003358244,0.0002863299,0.0005766233,0.0031319375,0.00059564546,0.13826537,0.01187533,0.062010515,0.13910525],"study_design_scores_gemma":[0.00005254393,0.00006791563,0.9416375,0.000025009653,0.000040953266,0.00033990672,0.00031577604,0.00091874076,0.007438635,0.0008690855,0.048265446,0.000028526585],"about_ca_topic_score_codex":0.010739757,"about_ca_topic_score_gemma":0.024449762,"teacher_disagreement_score":0.010739757,"about_ca_system_score_codex":0.00048038468,"about_ca_system_score_gemma":0.00050064456,"threshold_uncertainty_score":0.021354437},"labels":[],"label_agreement":null},{"id":"W2136971800","doi":"10.1086/519310","title":"Feedback and Its Feedback Effect on Feedback: Photoionization Suppression and Its Impact on Galactic Outflows","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Reionization; Astrophysics; Photoionization; Intergalactic medium; Galaxy; Halo; Radiative transfer; Dark Ages; Astronomy; Outflow; Universe; Active galactic nucleus; Redshift; Ionization; Ion","score_opus":0.006317210712455566,"score_gpt":0.24197528155612144,"score_spread":0.23565807084366588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136971800","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965706,0.00028812693,0.0016724019,0.00008992708,0.000006974717,0.0000041247295,0.000060654256,0.000032897144,0.0012742059],"genre_scores_gemma":[0.9996836,0.000046951995,0.000090101894,0.000007747379,0.0000041930393,0.0000011949284,0.000012890945,0.0000029509708,0.00015034643],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998758,0.000028034754,0.0000055791293,0.000019225734,0.000022281982,0.000049048205],"domain_scores_gemma":[0.9983999,0.00074326666,0.00035706468,0.0001098445,0.00012147551,0.00026834852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021975192,0.0007299828,0.00039057483,0.0002495516,0.00023361003,0.00054802565,0.00040646168,0.0004838085,0.0017845884],"category_scores_gemma":[0.0020536839,0.00014197029,0.0003478218,0.00014148297,0.00047087335,0.00047371973,0.00074654917,0.00028910273,0.0001693565],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022589616,0.0004354829,0.17230229,0.00032738637,0.00027261782,0.0021159647,0.0002812362,0.24186593,0.5427548,0.009349622,0.00044883724,0.02758683],"study_design_scores_gemma":[0.00036012798,0.0014176787,0.28589523,0.00006436457,0.00047743204,0.00095258345,0.00028896503,0.5452423,0.15029366,0.013383919,0.0015389466,0.0000847122],"about_ca_topic_score_codex":0.0025004263,"about_ca_topic_score_gemma":0.0009757478,"teacher_disagreement_score":0.0025004263,"about_ca_system_score_codex":0.0003635894,"about_ca_system_score_gemma":0.00022859473,"threshold_uncertainty_score":0.005970061},"labels":[],"label_agreement":null},{"id":"W2136997435","doi":"10.1086/421868","title":"Microlensing of the Broad Emission Line Region in the Quadruple Lens SDSS J1004+4112","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Gravitational microlensing; Quasar; Emission spectrum; Line (geometry); Spectroscopy; Lens (geology); Plane (geometry); Line-of-sight","score_opus":0.01102405077685898,"score_gpt":0.2200774255581738,"score_spread":0.20905337478131483,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2136997435","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992157,0.00004856083,0.00015323357,0.00001574837,0.0000023103862,0.0000030731749,0.00011827858,0.000033501557,0.0004095871],"genre_scores_gemma":[0.9986297,0.000030110465,0.0004140995,0.000016922379,0.0000048852694,0.000004702044,0.0005419307,0.0000092058835,0.0003483891],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984515,0.000009270642,0.0000067972073,0.00004414214,0.00004227066,0.000052313815],"domain_scores_gemma":[0.9994394,0.000041976058,0.00017474554,0.000056134668,0.0000617727,0.00022601224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023821396,0.00037429022,0.000297318,0.0016772522,0.0005047298,0.0005893189,0.00028476492,0.00039127786,0.0011956362],"category_scores_gemma":[0.0005951872,0.00034059846,0.0002587632,0.00058350066,0.00025985995,0.0003068074,0.00096133514,0.0003978056,0.00024736137],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037474395,0.00017526666,0.62299925,0.00005575939,0.00018789849,0.0011606779,0.00057803857,0.0018619373,0.35382378,0.00036774462,0.0006709344,0.017743923],"study_design_scores_gemma":[0.000010405405,0.00005866181,0.9911034,0.0000041308926,0.000024428009,0.0003379794,0.00012140169,0.0017239291,0.0057964623,0.00009880728,0.0007015335,0.000018723784],"about_ca_topic_score_codex":0.007125354,"about_ca_topic_score_gemma":0.017653532,"teacher_disagreement_score":0.007125354,"about_ca_system_score_codex":0.00078445993,"about_ca_system_score_gemma":0.00022590367,"threshold_uncertainty_score":0.014167726},"labels":[],"label_agreement":null},{"id":"W2137092421","doi":"10.1086/431743","title":"Constraints on the Orbital Evolution of Triton","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Orbital elements; Context (archaeology); Space debris; Astrophysics; Orbit (dynamics); Satellite; Orbital mechanics; Astronomy; Spacecraft; Geology; Aerospace engineering","score_opus":0.008269373844953071,"score_gpt":0.20799556269804964,"score_spread":0.19972618885309656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137092421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.982864,0.000113087015,0.004096772,0.00024359867,0.000020186057,0.000016074215,0.0004644011,0.00009027733,0.012091611],"genre_scores_gemma":[0.99791735,0.00006735986,0.001053787,0.00003074996,0.0000049410914,0.000012455117,0.0004223737,0.000028612843,0.00046225826],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999081,0.000017758797,0.000005422122,0.000014252186,0.000018172412,0.00003641999],"domain_scores_gemma":[0.9988839,0.0006292852,0.00013682566,0.00010361163,0.00011873503,0.00012762885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035846996,0.00040501257,0.00054345466,0.00036286033,0.0009534364,0.0010723962,0.00063266396,0.00051498506,0.0027351466],"category_scores_gemma":[0.003442981,0.00026344595,0.000417103,0.00032910376,0.0006061618,0.001234535,0.00078620366,0.00077140424,0.00028125805],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002570597,0.00008993214,0.027758457,0.00004628065,0.000072961346,0.00027233822,0.00013858339,0.9539981,0.0024594592,0.010302043,0.0011140885,0.0034907744],"study_design_scores_gemma":[0.000073753166,0.00006189128,0.0036194432,0.000012411415,0.000025307188,0.00004356386,0.0000967413,0.99074966,0.0009776304,0.0034823036,0.0008402814,0.000017015445],"about_ca_topic_score_codex":0.017227756,"about_ca_topic_score_gemma":0.013583134,"teacher_disagreement_score":0.017227756,"about_ca_system_score_codex":0.0007996027,"about_ca_system_score_gemma":0.0008128199,"threshold_uncertainty_score":0.03425497},"labels":[],"label_agreement":null},{"id":"W2137114988","doi":"10.1088/0004-637x/732/1/12","title":"EARLY-TYPE GALAXIES AT<i>z</i>∼ 1.3. II. MASSES AND AGES OF EARLY-TYPE GALAXIES IN DIFFERENT ENVIRONMENTS AND THEIR DEPENDENCE ON STELLAR POPULATION MODEL ASSUMPTIONS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Australian Research Council; Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Galaxy; Stellar mass; Supercluster (genetic); Stellar population; Galaxy cluster; Redshift; Population; Field galaxy","score_opus":0.0188209650549356,"score_gpt":0.21174355147384985,"score_spread":0.19292258641891424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137114988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975273,0.00015356811,0.0006623695,0.000012501087,0.0000013396592,0.000004369532,0.0007602122,0.000021757605,0.00085661287],"genre_scores_gemma":[0.99758863,0.00008401898,0.0005496934,0.0000063549605,0.0000025517786,0.000005423367,0.0015661974,0.000008304595,0.00018896307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998319,0.000024800682,0.000012420775,0.00006084509,0.000025243375,0.000044769004],"domain_scores_gemma":[0.9989832,0.0003370184,0.00031044584,0.0001278138,0.00013033097,0.00011121994],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067571434,0.00030043127,0.0002546971,0.0008810036,0.00024372083,0.00073177076,0.00044618096,0.00026433638,0.0011019795],"category_scores_gemma":[0.0014058669,0.0001614996,0.00034332767,0.00043058934,0.00020866988,0.0006683341,0.00042617662,0.0003205625,0.00038385144],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016404831,0.000020248039,0.98803174,0.000027637965,0.000037539376,0.00006948403,0.00014347969,0.0037858237,0.003440319,0.0003563417,0.00007825751,0.0038450933],"study_design_scores_gemma":[0.000003977016,0.000034394827,0.9930773,0.000008364745,0.000018036635,0.000073183226,0.000085092375,0.0038680274,0.0021333387,0.00032854237,0.00036443849,0.0000053746867],"about_ca_topic_score_codex":0.004940976,"about_ca_topic_score_gemma":0.0061443844,"teacher_disagreement_score":0.004940976,"about_ca_system_score_codex":0.0006314119,"about_ca_system_score_gemma":0.00010818669,"threshold_uncertainty_score":0.009824455},"labels":[],"label_agreement":null},{"id":"W2137189780","doi":"10.1086/432247","title":"Galactic Bulge Microlensing Events from the MACHO Collaboration","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gravitational microlensing; Astrophysics; Physics; Bulge; Stars; Astronomy; Galactic Center; Sagittarius; Galaxy; Sagittarius A*; Extinction (optical mineralogy); Milky Way","score_opus":0.008414914863753965,"score_gpt":0.22708301040343737,"score_spread":0.21866809553968342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137189780","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94630855,0.0017965913,0.0006985254,0.00014353101,0.000023204442,0.00006465607,0.041609965,0.0002591823,0.009095761],"genre_scores_gemma":[0.8793036,0.00087460363,0.0020891502,0.00014407864,0.00007213568,0.00006629865,0.115099944,0.00007527582,0.0022749263],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993155,0.00007095992,0.00007966028,0.00016212834,0.00022987266,0.00014183548],"domain_scores_gemma":[0.99875164,0.00009987723,0.00046900913,0.00017989754,0.00014352945,0.0003559944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044649836,0.0003419143,0.0003109874,0.0032835293,0.00040528853,0.00071468495,0.00035946356,0.00021867426,0.002369424],"category_scores_gemma":[0.0014019802,0.00016445934,0.00027526284,0.0023155657,0.000095643554,0.00036185625,0.0012273788,0.00017200512,0.00085172587],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003264468,0.000045963512,0.9444729,0.00010935261,0.00015344641,0.00052628544,0.00055177,0.00018272153,0.0023151229,0.00028881934,0.012337981,0.03868917],"study_design_scores_gemma":[0.000016720001,0.00003688519,0.97988737,0.000019562787,0.00003767684,0.0012196207,0.00015114622,0.00028094475,0.0008439257,0.00009070896,0.01740557,0.000009925233],"about_ca_topic_score_codex":0.005234664,"about_ca_topic_score_gemma":0.011129048,"teacher_disagreement_score":0.005234664,"about_ca_system_score_codex":0.00034756344,"about_ca_system_score_gemma":0.00019650314,"threshold_uncertainty_score":0.0104084015},"labels":[],"label_agreement":null},{"id":"W2137201296","doi":"10.1088/0004-637x/718/2/1200","title":"A<i>SPITZER</i>c2d LEGACY SURVEY TO IDENTIFY AND CHARACTERIZE DISKS WITH INNER DUST HOLES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; Planet; Photometry (optics); Astronomy; Stars; Exoplanet; Planetary system; Brown dwarf; Spectral line; Spectral energy distribution; Population; Galaxy","score_opus":0.014635313151094603,"score_gpt":0.26362407103993435,"score_spread":0.24898875788883976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137201296","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9500513,0.00033490628,0.0011535566,0.0001417051,0.0000150001,0.00017180873,0.036860745,0.00022318252,0.011047904],"genre_scores_gemma":[0.92004514,0.00041751104,0.0047240905,0.00024722735,0.00005303152,0.00023528768,0.069540136,0.000059756723,0.004677769],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982303,0.000008141113,0.0000152053935,0.000038852264,0.00006835739,0.000046298555],"domain_scores_gemma":[0.99893206,0.000050596274,0.0003502074,0.00011842354,0.0003360997,0.00021268477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034583794,0.00027325493,0.000182098,0.0047117188,0.00050092663,0.00044555703,0.00039062413,0.00017373404,0.0026298787],"category_scores_gemma":[0.0005301173,0.00008848524,0.00019236005,0.0025982836,0.00013852447,0.00031920543,0.0006740967,0.00018466215,0.0013597368],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003611197,0.000046232377,0.9740457,0.00004033229,0.000030193463,0.00013820641,0.00022040989,0.00015550751,0.005325277,0.00013308901,0.006990235,0.012838703],"study_design_scores_gemma":[0.0000024578367,0.000011712138,0.9941202,0.0000061039154,0.0000063669404,0.0000960763,0.00009164885,0.00018595751,0.00059718004,0.000016659294,0.004863555,0.0000020833743],"about_ca_topic_score_codex":0.025631743,"about_ca_topic_score_gemma":0.051611323,"teacher_disagreement_score":0.025631743,"about_ca_system_score_codex":0.0005584733,"about_ca_system_score_gemma":0.0004605822,"threshold_uncertainty_score":0.05096513},"labels":[],"label_agreement":null},{"id":"W2137337429","doi":"10.1086/345787","title":"Can White Dwarf Asteroseismology Really Constrain the [TSUP]12[/TSUP]C(α, γ)[TSUP]16[/TSUP]O Reaction Rate?","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Asteroseismology; Physics; White dwarf; Astrophysics; Diffusion; Effective temperature; Core (optical fiber); Stellar evolution; Star (game theory); Stars; Thermodynamics; Optics","score_opus":0.014739534351337727,"score_gpt":0.2138370907356149,"score_spread":0.19909755638427717,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137337429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97736984,0.0007419216,0.016042097,0.00044949315,0.000049056824,0.00001105219,0.0003356943,0.00015809904,0.004842721],"genre_scores_gemma":[0.997512,0.00027392062,0.0016964849,0.00006038346,0.00001007429,0.0000029430078,0.00017024428,0.000043122105,0.00023084562],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998312,0.000028604034,0.000013913159,0.0000669314,0.00002769428,0.000031601387],"domain_scores_gemma":[0.9992374,0.00022895311,0.00020375109,0.00016660569,0.00010464448,0.00005873585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012199531,0.00060193404,0.0005734452,0.00052536646,0.00027429877,0.0010741267,0.00067543786,0.0006522441,0.0010139404],"category_scores_gemma":[0.004031057,0.0003751032,0.00040665138,0.0005307485,0.000540414,0.0019905914,0.0005115521,0.0004942038,0.00043024978],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005206718,0.00007026486,0.738121,0.00045241867,0.00040469278,0.0004181966,0.0004636398,0.052284922,0.15558596,0.01513065,0.00088266976,0.035665065],"study_design_scores_gemma":[0.00012028023,0.00036312183,0.5431195,0.00010162291,0.00044373114,0.0009732688,0.0014186715,0.2512398,0.13323985,0.04520975,0.023573274,0.0001970375],"about_ca_topic_score_codex":0.006976169,"about_ca_topic_score_gemma":0.005723212,"teacher_disagreement_score":0.006976169,"about_ca_system_score_codex":0.00053485675,"about_ca_system_score_gemma":0.000372898,"threshold_uncertainty_score":0.013871074},"labels":[],"label_agreement":null},{"id":"W2137364917","doi":"10.1088/0004-637x/789/1/59","title":"ACCRETING PLANETS AS DUST DAMS IN “TRANSITION” DISKS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Accretion (finance); Radiation pressure; Accretion disc; Luminosity; Planetary mass","score_opus":0.008458669697668002,"score_gpt":0.24452306370490004,"score_spread":0.23606439400723203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137364917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998645,0.000036801415,0.00062145357,0.000015977263,0.000001053423,0.0000020882158,0.000012098979,0.000019046332,0.0006464439],"genre_scores_gemma":[0.9996246,0.000017680297,0.00023377655,0.0000047012645,0.0000014187798,0.0000013997172,0.000017881031,0.0000026256469,0.00009581077],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999442,0.000009934012,0.000002745657,0.000014449851,0.0000074616837,0.000021161859],"domain_scores_gemma":[0.99968207,0.00008474268,0.000098587036,0.000026910331,0.000019881,0.00008783787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011135601,0.0001061542,0.00014264102,0.00032745753,0.00044485147,0.0008115411,0.0003668126,0.0003421349,0.0008070259],"category_scores_gemma":[0.0008036654,0.00014418588,0.00015922284,0.00018340573,0.000482087,0.00067791034,0.0006942979,0.00024425212,0.00013490244],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015957733,0.00029813894,0.69133973,0.00018391908,0.00016569988,0.010360565,0.0052832454,0.064623185,0.1509169,0.047854118,0.0009838449,0.026394801],"study_design_scores_gemma":[0.00022482092,0.0011424193,0.5978622,0.000059793052,0.00023499956,0.004608312,0.0073443046,0.2876347,0.03910549,0.05087174,0.010807332,0.000103855855],"about_ca_topic_score_codex":0.0013010337,"about_ca_topic_score_gemma":0.0009566297,"teacher_disagreement_score":0.0013010337,"about_ca_system_score_codex":0.0003233933,"about_ca_system_score_gemma":0.00012885922,"threshold_uncertainty_score":0.0026997328},"labels":[],"label_agreement":null},{"id":"W2137384184","doi":"10.1086/590908","title":"PSR J1856+0245: Arecibo Discovery of a Young, Energetic Pulsar Coincident with the TeV γ-Ray Source HESS J1857+026","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; Fonds Québécois de la Recherche sur la Nature et les Technologies; McGill University; Canadian Space Agency; National Science Foundation","keywords":"Pulsar; Physics; Pulsar wind nebula; Astrophysics; Astronomy; Pulsar planet; Luminosity; Vela; Nebula; Binary pulsar; Millisecond pulsar; Galaxy; Stars","score_opus":0.00965697542506536,"score_gpt":0.26437603756401346,"score_spread":0.25471906213894807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137384184","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99712735,0.00017483978,0.00012329657,0.000047393925,0.0000098568635,0.000008351391,0.00018343404,0.000017512739,0.0023080185],"genre_scores_gemma":[0.9983011,0.00012483986,0.00032742176,0.00007298608,0.000023143517,0.0000054194616,0.00070385856,0.0000044601047,0.00043687655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999043,0.000007643092,0.000004388833,0.000028348397,0.00002687899,0.000028544266],"domain_scores_gemma":[0.9998011,0.000011737174,0.00007507663,0.000022737942,0.000021003105,0.00006840037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016193984,0.0002084734,0.00018360678,0.0006059969,0.00045518504,0.00063933,0.00021982485,0.00030430302,0.001073919],"category_scores_gemma":[0.00025809745,0.00010914008,0.00013272022,0.0006366164,0.0002680432,0.00018862993,0.000636324,0.00019558404,0.00027941412],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044214126,0.00015432636,0.90779364,0.00010001683,0.00013932415,0.0054832203,0.0006877899,0.00023545382,0.05331734,0.0008557667,0.002283953,0.028507052],"study_design_scores_gemma":[0.000020340596,0.00006686263,0.98995423,0.000008941523,0.000026903926,0.0019448118,0.00012980375,0.00016282465,0.0013447552,0.000064446845,0.006271434,0.0000046804034],"about_ca_topic_score_codex":0.004847884,"about_ca_topic_score_gemma":0.007475485,"teacher_disagreement_score":0.004847884,"about_ca_system_score_codex":0.00035626773,"about_ca_system_score_gemma":0.00015908627,"threshold_uncertainty_score":0.009639323},"labels":[],"label_agreement":null},{"id":"W2137507016","doi":"10.1088/0004-637x/807/2/138","title":"Chitah: STRONG-GRAVITATIONAL-LENS HUNTER IN IMAGING SURVEYS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Quasar; Gravitational lens; Lens (geology); Einstein radius; Galaxy; Telescope; Large Synoptic Survey Telescope","score_opus":0.015020752243671614,"score_gpt":0.23981435281359337,"score_spread":0.22479360056992176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137507016","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.28088647,0.0009671578,0.52087975,0.00093525834,0.00044382102,0.0015611524,0.007609549,0.17557484,0.011142054],"genre_scores_gemma":[0.42855057,0.0001598323,0.55681694,0.0004935253,0.00011869982,0.00096947857,0.007222839,0.0018297036,0.003838436],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9985417,0.0003593795,0.00004897669,0.00041487746,0.0004203702,0.00021486395],"domain_scores_gemma":[0.9958891,0.0015651745,0.00046813616,0.0009988486,0.00044349636,0.0006352108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027438747,0.0009976513,0.00074942544,0.0012292484,0.0006781701,0.00079525384,0.00309786,0.0016157205,0.0029860924],"category_scores_gemma":[0.008748439,0.0008315777,0.00081399037,0.0011028217,0.00094180036,0.0015668231,0.0028704323,0.0016321051,0.0020819213],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022109884,0.0009253982,0.24713117,0.0009378588,0.00075812265,0.001080539,0.0011957614,0.1541641,0.03924926,0.014728021,0.13287085,0.40474784],"study_design_scores_gemma":[0.00031036304,0.00043234823,0.02398281,0.000043604494,0.000067183544,0.000432123,0.00017943724,0.9246951,0.014436761,0.008372885,0.02694106,0.00010639215],"about_ca_topic_score_codex":0.0065002525,"about_ca_topic_score_gemma":0.010590082,"teacher_disagreement_score":0.0065002525,"about_ca_system_score_codex":0.00066006865,"about_ca_system_score_gemma":0.001679199,"threshold_uncertainty_score":0.014511168},"labels":[],"label_agreement":null},{"id":"W2137520608","doi":"10.1088/0004-637x/804/2/95","title":"ON SHOCKS DRIVEN BY HIGH-MASS PLANETS IN RADIATIVELY INEFFICIENT DISKS. I. TWO-DIMENSIONAL GLOBAL DISK SIMULATIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Protoplanet; Physics; Planet; Astrophysics; Adiabatic process; Spiral galaxy; Spiral (railway); Gas giant; Exoplanet; Stars; Protoplanetary disk","score_opus":0.011429756038131842,"score_gpt":0.2575120117844094,"score_spread":0.24608225574627757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137520608","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98971903,0.00012338835,0.0029433277,0.00026277875,0.000034220608,0.000055480457,0.0008032625,0.00012224031,0.005936388],"genre_scores_gemma":[0.9947761,0.00011139357,0.0025769877,0.0001372466,0.000020797657,0.00007383937,0.0009746291,0.00005622698,0.0012726133],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999814,0.000046631805,0.000009417957,0.000024740188,0.000030457026,0.0000747692],"domain_scores_gemma":[0.9988852,0.0005551587,0.00013059188,0.000058385704,0.00013754291,0.00023304156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046456564,0.0008728357,0.0010540265,0.0008131442,0.00084721093,0.0012202563,0.0014708877,0.0018278222,0.00283576],"category_scores_gemma":[0.0023058206,0.0004629931,0.00095189194,0.0006654349,0.0013207374,0.0008408489,0.0012137555,0.0014291628,0.00023436944],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019174279,0.00011991716,0.0066222055,0.000031492542,0.000041225812,0.00017785696,0.00008042561,0.98958814,0.0008591722,0.0013545536,0.00028204828,0.00065114134],"study_design_scores_gemma":[0.00006616723,0.000041238163,0.0015173813,0.000006233517,0.0000062846425,0.000011233243,0.00005427316,0.9975694,0.00019141467,0.00039950304,0.00012928774,0.0000075821067],"about_ca_topic_score_codex":0.029765911,"about_ca_topic_score_gemma":0.015197917,"teacher_disagreement_score":0.029765911,"about_ca_system_score_codex":0.0015164547,"about_ca_system_score_gemma":0.00088540453,"threshold_uncertainty_score":0.059185266},"labels":[],"label_agreement":null},{"id":"W2137800231","doi":"10.1088/0004-637x/709/1/159","title":"WASP-17b: AN ULTRA-LOW DENSITY PLANET IN A PROBABLE RETROGRADE ORBIT","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":218,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Queen's University; Queen's University Belfast","keywords":"Planet; Physics; Orbital eccentricity; Astronomy; Astrophysics; Orbit (dynamics); RADIUS; Exoplanet; Circular orbit; Jupiter (rocket family); Tidal heating; Eccentricity (behavior); Eclipse; Surface gravity; Stars","score_opus":0.009619611074860928,"score_gpt":0.21946574741125993,"score_spread":0.209846136336399,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137800231","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98534375,0.004022025,0.0018085516,0.00061677664,0.0002363802,0.000026946707,0.0009310687,0.00015703097,0.006857562],"genre_scores_gemma":[0.98897225,0.0012504765,0.0024938046,0.00017726904,0.00012582322,0.000012492643,0.0028362616,0.00003933604,0.004092418],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998739,0.0000066916928,0.000004795605,0.000042988362,0.000031924494,0.000039719765],"domain_scores_gemma":[0.99976975,0.000018203544,0.00005719203,0.000028194632,0.000025162371,0.00010148989],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015280841,0.0004906195,0.00035723706,0.0010017081,0.0012417111,0.0012049237,0.0006584542,0.0011792858,0.0017041018],"category_scores_gemma":[0.00034683474,0.00023206712,0.00029865268,0.00074061466,0.0007422896,0.00050922955,0.0009665784,0.0007240753,0.0021888244],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015730801,0.00026941067,0.3624105,0.00075515587,0.00026968442,0.08414643,0.001101596,0.0010074268,0.45769188,0.0090621915,0.01187708,0.069835596],"study_design_scores_gemma":[0.0001323069,0.0016267797,0.21317457,0.0002895258,0.0003460418,0.20310718,0.0017709814,0.0052258926,0.21571356,0.006676775,0.35180664,0.00012968936],"about_ca_topic_score_codex":0.001190042,"about_ca_topic_score_gemma":0.0010389948,"teacher_disagreement_score":0.0017041018,"about_ca_system_score_codex":0.00044684537,"about_ca_system_score_gemma":0.0002251794,"threshold_uncertainty_score":0.005700767},"labels":[],"label_agreement":null},{"id":"W2137827055","doi":"10.1088/0004-637x/761/1/22","title":"REDSHIFTS, SAMPLE PURITY, AND BCG POSITIONS FOR THE GALAXY CLUSTER CATALOG FROM THE FIRST 720 SQUARE DEGREES OF THE SOUTH POLE TELESCOPE SURVEY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Redshift; Physics; Astrophysics; Galaxy; South Pole Telescope; Galaxy cluster; Cluster (spacecraft); Telescope; Estimator; Cluster sampling; Brightest cluster galaxy; Astronomy; Population; Statistics","score_opus":0.01596515801466389,"score_gpt":0.2232387540398959,"score_spread":0.20727359602523202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2137827055","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99337876,0.00015907772,0.0005080661,0.000044910477,0.0000032293783,0.000017379794,0.0044970475,0.00006666507,0.0013249317],"genre_scores_gemma":[0.9902722,0.000088333945,0.00063061033,0.000015697933,0.0000103622115,0.000027025324,0.008302022,0.000029235558,0.0006244236],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99930716,0.00009443904,0.000039894985,0.00019490875,0.00023097232,0.00013259528],"domain_scores_gemma":[0.9976591,0.00048251706,0.0006971381,0.0005540671,0.00030993237,0.0002972557],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010313409,0.00022072588,0.0003919071,0.0033631185,0.00051340665,0.00077575573,0.00038167703,0.00024934945,0.0032415972],"category_scores_gemma":[0.003690047,0.0001554763,0.00022965905,0.0019770975,0.00034886558,0.00028911897,0.0006593255,0.0002482109,0.0010192348],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009110978,0.000015195366,0.99012285,0.000014982855,0.000040136103,0.000032447522,0.00020139047,0.0004040677,0.0015329164,0.00015391127,0.0010501064,0.006340923],"study_design_scores_gemma":[0.0000045144675,0.000012785947,0.9985671,0.0000017410864,0.000009271852,0.000044105687,0.00004439853,0.00038780578,0.00019204279,0.00003273049,0.0007012525,0.0000022445822],"about_ca_topic_score_codex":0.013748488,"about_ca_topic_score_gemma":0.028364273,"teacher_disagreement_score":0.013748488,"about_ca_system_score_codex":0.0004900729,"about_ca_system_score_gemma":0.00029499733,"threshold_uncertainty_score":0.027336955},"labels":[],"label_agreement":null},{"id":"W2138063964","doi":"10.1086/427184","title":"A Period and a Prediction for the Of?p Spectrum Alternator HD 191612","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Light curve; Rotation period; Orbital period; Period (music); Spectral line; Orbit (dynamics); Emission spectrum; Orbital eccentricity; Rotation (mathematics)","score_opus":0.008365525468450673,"score_gpt":0.21594948913424486,"score_spread":0.20758396366579418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138063964","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9718615,0.0005420695,0.0039237062,0.0012933329,0.00019529917,0.000027521417,0.0006692369,0.00009497801,0.02139226],"genre_scores_gemma":[0.99812835,0.00009272725,0.00056044006,0.00011158257,0.00008315125,0.00000960553,0.0004642327,0.000014183738,0.0005357335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999008,0.0000118105245,0.000006791365,0.00004062546,0.000014928521,0.000025073583],"domain_scores_gemma":[0.99955827,0.00008531054,0.00013963968,0.00006542521,0.00006864878,0.00008268408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002501603,0.00024489037,0.00012671105,0.00040295706,0.000503836,0.0009627384,0.00045986447,0.0006291493,0.0033018072],"category_scores_gemma":[0.0012981731,0.0001444012,0.00024011185,0.0002435257,0.00035046317,0.00069203106,0.00043130104,0.0006024879,0.0011021553],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018942391,0.00022030347,0.828299,0.000192692,0.00008007998,0.0028849614,0.00066701794,0.0037495098,0.06527148,0.032240644,0.007820615,0.0566795],"study_design_scores_gemma":[0.00008731304,0.00028036477,0.9467391,0.000036757516,0.00004089534,0.0020246147,0.0005003949,0.010931809,0.0058674887,0.019582722,0.013872712,0.000035841676],"about_ca_topic_score_codex":0.00082220143,"about_ca_topic_score_gemma":0.0006913056,"teacher_disagreement_score":0.0033018072,"about_ca_system_score_codex":0.0003321923,"about_ca_system_score_gemma":0.00017844426,"threshold_uncertainty_score":0.011045635},"labels":[],"label_agreement":null},{"id":"W2138187979","doi":"10.1088/0004-637x/735/2/95","title":"THE UNUSUAL X-RAY BINARIES OF THE GLOBULAR CLUSTER NGC 6652","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Photon; Spectral line; Accretion (finance); Power law; Cluster (spacecraft); Polar; Astronomy; Galaxy; Optics","score_opus":0.015816498630863502,"score_gpt":0.21447527771446412,"score_spread":0.1986587790836006,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138187979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99761707,0.00022482115,0.00008895661,0.000033565808,0.000005654294,0.000004560682,0.00029969448,0.00002295935,0.0017026424],"genre_scores_gemma":[0.99900204,0.000057539786,0.0001498167,0.000016313235,0.000006168095,0.0000018525562,0.00036976396,0.000003517724,0.00039296],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983704,0.000009728526,0.000009864384,0.000045419372,0.00003749388,0.00006029325],"domain_scores_gemma":[0.99976176,0.000012565263,0.00007657167,0.00002578259,0.000016668333,0.00010675148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012697533,0.00033314154,0.0002383678,0.0009601996,0.000743253,0.0006278453,0.00031216344,0.0002910891,0.0018325478],"category_scores_gemma":[0.00035970545,0.0002586717,0.00013443707,0.0009309873,0.00030697885,0.00039388693,0.0007868673,0.0002104526,0.0004744758],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049624185,0.000080321166,0.93495363,0.00006208906,0.00007451802,0.0033496164,0.00067741435,0.00071235,0.042702623,0.0016430083,0.0020538683,0.013194304],"study_design_scores_gemma":[0.0000053461604,0.000024975228,0.99696594,0.0000052604855,0.0000069176212,0.0010334983,0.000076592965,0.00032486898,0.00027260557,0.0001279895,0.0011486629,0.0000073939227],"about_ca_topic_score_codex":0.014612455,"about_ca_topic_score_gemma":0.02846528,"teacher_disagreement_score":0.014612455,"about_ca_system_score_codex":0.0005340437,"about_ca_system_score_gemma":0.00017080062,"threshold_uncertainty_score":0.02905482},"labels":[],"label_agreement":null},{"id":"W2138226510","doi":"10.1088/0004-637x/790/1/39","title":"A STATE CHANGE IN THE MISSING LINK BINARY PULSAR SYSTEM PSR J1023+0038","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":227,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; U.S. Department of Energy; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Radio Astronomy Observatory; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; National Science Foundation","keywords":"Pulsar; Millisecond pulsar; Physics; Astrophysics; Neutron star; Astronomy; Accretion (finance); Pulsar planet; Binary number; Millisecond; Low Mass; Binary pulsar; Binary system; Stars","score_opus":0.022945124155124598,"score_gpt":0.25010505909159175,"score_spread":0.22715993493646716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138226510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992699,0.00003059076,0.000075853866,0.0000128976835,0.0000025115528,0.0000015628799,0.000036321468,0.000010115874,0.0005602843],"genre_scores_gemma":[0.99957365,0.000016947213,0.000108067296,0.000006134761,0.0000023130374,0.0000021274425,0.00009371864,0.0000019008173,0.00019517056],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999967,0.000003767445,0.0000023126415,0.000010652639,0.000008112195,0.000008252858],"domain_scores_gemma":[0.99988234,0.000018047147,0.000055880348,0.000017958248,0.000009454238,0.000016287795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006802685,0.00010027367,0.000136742,0.00014847731,0.00025945046,0.00030393884,0.00016095598,0.00016783252,0.0013422046],"category_scores_gemma":[0.00043875416,0.000071520015,0.000048592974,0.00018744232,0.0002455066,0.00024655726,0.00028753915,0.00023870621,0.00020636049],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017723418,0.00040797013,0.31288192,0.00018586004,0.00009720679,0.0030059088,0.0013047481,0.0039192857,0.62219477,0.0034023977,0.0012234309,0.049604148],"study_design_scores_gemma":[0.00010969317,0.0015112103,0.9155433,0.000017720808,0.00006826591,0.0032790424,0.0008149248,0.019152386,0.051138647,0.0030510146,0.005268047,0.00004577792],"about_ca_topic_score_codex":0.0007481342,"about_ca_topic_score_gemma":0.0008330303,"teacher_disagreement_score":0.0013422046,"about_ca_system_score_codex":0.00017245246,"about_ca_system_score_gemma":0.00008653215,"threshold_uncertainty_score":0.004490137},"labels":[],"label_agreement":null},{"id":"W2138334435","doi":"10.1088/0004-637x/763/2/102","title":"NONLINEAR EVOLUTION OF RAYLEIGH-TAYLOR INSTABILITY IN A RADIATION-SUPPORTED ATMOSPHERE","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Laser-Plasma Interactions and Diagnostics","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Opacity; Instability; Radiation; Radiation pressure; Scattering; Anisotropy; Radiative transfer; Tensor (intrinsic definition)","score_opus":0.00614375633556077,"score_gpt":0.227665813337505,"score_spread":0.22152205700194422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138334435","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941369,0.00005029322,0.0032750075,0.00008312132,0.0000099204035,0.0000146567645,0.000055179433,0.000050712475,0.0023242445],"genre_scores_gemma":[0.99763536,0.000025971884,0.0018723401,0.000013239193,0.000004046607,0.000010108789,0.000042240114,0.000015051728,0.00038162235],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999043,0.000021371061,0.0000057410703,0.00001576295,0.000021705724,0.000031166826],"domain_scores_gemma":[0.99955887,0.00015240724,0.00011822073,0.000029377357,0.000049971044,0.00009114522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024245765,0.00038740446,0.00037246168,0.00041735475,0.00062604796,0.0007056335,0.0005562455,0.0007339837,0.0008459533],"category_scores_gemma":[0.0012910793,0.00023609372,0.0005395653,0.00023067291,0.00093629665,0.0005257632,0.0008285239,0.00052568456,0.000079517486],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026950528,0.00016338982,0.02042436,0.000073912364,0.00007689042,0.00083651557,0.00040331142,0.92036694,0.04562094,0.008040431,0.0003424868,0.0033813985],"study_design_scores_gemma":[0.000032916483,0.000049436876,0.002284138,0.000004095716,0.0000063004795,0.000041866442,0.000039574894,0.9952128,0.0017673376,0.00044414424,0.00010779795,0.000009645154],"about_ca_topic_score_codex":0.008644946,"about_ca_topic_score_gemma":0.0030462588,"teacher_disagreement_score":0.008644946,"about_ca_system_score_codex":0.00076597417,"about_ca_system_score_gemma":0.00052320637,"threshold_uncertainty_score":0.017189264},"labels":[],"label_agreement":null},{"id":"W2138354370","doi":"10.1086/519546","title":"The Formation of Globular Cluster Systems in Massive Elliptical Galaxies: Globular Cluster Multimodality from Radial Variation of Stellar Populations","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Elliptical galaxy; Star cluster; Cluster (spacecraft); Galaxy cluster; Galaxy; Horizontal branch","score_opus":0.010640957075177829,"score_gpt":0.23185784248203056,"score_spread":0.22121688540685275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138354370","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960438,0.00039746752,0.00076379103,0.00028415857,0.000027195021,0.000008268227,0.00047884812,0.00003736068,0.001959144],"genre_scores_gemma":[0.9986651,0.00011673994,0.0002219141,0.000019262652,0.00005245908,0.0000032507396,0.00034246003,0.000014949653,0.00056383474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971694,0.000049789418,0.000016691209,0.00008669791,0.000084767045,0.00004515872],"domain_scores_gemma":[0.993569,0.002299087,0.0014901621,0.0003984816,0.0012516608,0.0009915918],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010021391,0.00017098148,0.00034755218,0.0016114922,0.00048642204,0.0012357886,0.000446007,0.00071115745,0.0058653774],"category_scores_gemma":[0.011194277,0.00034310875,0.00021884803,0.0009899244,0.000522354,0.0011356376,0.0009341669,0.0003841183,0.000999776],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029342395,0.000022973556,0.9541093,0.00013233084,0.00010340157,0.00026182775,0.0004909656,0.0012929611,0.012172249,0.0012581672,0.0028056416,0.027056795],"study_design_scores_gemma":[0.0000052040923,0.00001962087,0.99570066,0.000008997305,0.000020862559,0.00013566666,0.00013542235,0.0020553195,0.0005943498,0.00091955776,0.00038862403,0.000015623069],"about_ca_topic_score_codex":0.001513829,"about_ca_topic_score_gemma":0.0024331084,"teacher_disagreement_score":0.0058653774,"about_ca_system_score_codex":0.00029887084,"about_ca_system_score_gemma":0.00019469744,"threshold_uncertainty_score":0.01962161},"labels":[],"label_agreement":null},{"id":"W2138521688","doi":"10.1086/509495","title":"Formation of Narrow Dust Rings in Circumstellar Debris Disks","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Stars; Debris; Circumstellar dust; Astrophysics; Debris disk; Planet; Circumstellar disk; Cosmic dust; Instability; Planetary system; Mechanics; Meteorology","score_opus":0.011128786690683574,"score_gpt":0.24285285474451831,"score_spread":0.23172406805383475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138521688","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981286,0.00022671142,0.00076364574,0.000009266138,0.000002540377,0.0000029975606,0.00005818856,0.000024959825,0.00078314904],"genre_scores_gemma":[0.99943846,0.000045049885,0.0003374135,0.0000019652189,0.0000030637627,0.0000017081478,0.000052263116,0.0000033644553,0.000116626295],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999505,0.000005585461,0.000003595061,0.000015073685,0.00000885713,0.000016433014],"domain_scores_gemma":[0.9997191,0.000048995178,0.00013180215,0.000033281227,0.00001953471,0.000047234727],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011930845,0.00014905607,0.00014666367,0.0004605552,0.00023462233,0.0005721901,0.00022816943,0.0002454874,0.00089348777],"category_scores_gemma":[0.0004770083,0.00015727602,0.00018994148,0.00027567492,0.0002772908,0.0002859448,0.00028316703,0.00006914886,0.0001946243],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033715589,0.00008626668,0.85155046,0.000151591,0.00011970274,0.0020188822,0.0004190354,0.03228817,0.090873234,0.0027999375,0.00051429844,0.01884132],"study_design_scores_gemma":[0.000048442347,0.000139888,0.9251185,0.00001928766,0.0000854801,0.0013505938,0.00025096172,0.049669273,0.018498138,0.0018071485,0.0029917562,0.000020575122],"about_ca_topic_score_codex":0.0006476899,"about_ca_topic_score_gemma":0.0004793493,"teacher_disagreement_score":0.00089348777,"about_ca_system_score_codex":0.00021921663,"about_ca_system_score_gemma":0.0000735078,"threshold_uncertainty_score":0.0029889941},"labels":[],"label_agreement":null},{"id":"W2138540103","doi":"10.1088/0004-637x/727/2/105","title":"IDENTIFICATION OF A POPULATION OF X-RAY-EMITTING MASSIVE STARS IN THE GALACTIC PLANE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galactic plane; Stars; Observatory; Astronomy; Spectral line; Spectroscopy; Emission spectrum; Infrared; Binary number","score_opus":0.020763839977567197,"score_gpt":0.2382981467522833,"score_spread":0.2175343067747161,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138540103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991178,0.00008912663,0.00010502695,0.000008474401,0.0000016426134,0.000006109228,0.00006170784,0.00000527182,0.0006048586],"genre_scores_gemma":[0.99873203,0.00008317013,0.0003690876,0.00001667257,0.0000076377655,0.0000049791074,0.00041717337,0.000003262269,0.0003659655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998419,0.000010943492,0.0000128881675,0.00005394503,0.000050776365,0.000029481173],"domain_scores_gemma":[0.9996929,0.000007892447,0.00013570882,0.000022678183,0.00003222482,0.00010858498],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016856063,0.0002456108,0.0002919838,0.000826114,0.0005131189,0.0009754419,0.0003476221,0.00023332977,0.00082727545],"category_scores_gemma":[0.00024947812,0.00014514472,0.00011267644,0.00075653556,0.00024096959,0.00027754047,0.000590209,0.00019407098,0.00048723948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012227676,0.000058783735,0.96896017,0.0000132947625,0.000033963905,0.00031086424,0.00027586523,0.00011407648,0.023405785,0.00015689782,0.00012904116,0.006419006],"study_design_scores_gemma":[0.0000060954444,0.000076872166,0.99769294,0.0000031129393,0.000008370685,0.0005550717,0.00019785426,0.00019859208,0.0005918933,0.00004423141,0.0006227685,0.0000021939518],"about_ca_topic_score_codex":0.0026849334,"about_ca_topic_score_gemma":0.0048218304,"teacher_disagreement_score":0.0026849334,"about_ca_system_score_codex":0.00021428519,"about_ca_system_score_gemma":0.00012818103,"threshold_uncertainty_score":0.005338669},"labels":[],"label_agreement":null},{"id":"W2138598873","doi":"10.1088/0004-637x/748/2/136","title":"TOWARD EARLY-WARNING DETECTION OF GRAVITATIONAL WAVES FROM COMPACT BINARY COALESCENCE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":259,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Toronto Metropolitan University; Perimeter Institute; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Coalescence (physics); Gravitational wave; Binary number; Detector; Binary star; Binary Independence Model","score_opus":0.02360683591165543,"score_gpt":0.3104100226637387,"score_spread":0.2868031867520833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138598873","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.28614137,0.0002979331,0.7061277,0.0012206475,0.00011671089,0.000121213234,0.00017345152,0.0015558782,0.004245058],"genre_scores_gemma":[0.8104601,0.00010013992,0.18801033,0.00019302456,0.00007769004,0.000049027753,0.00016407206,0.0000680147,0.0008775288],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995047,0.00013736989,0.00002217154,0.00007788099,0.00019086915,0.000066986104],"domain_scores_gemma":[0.99432147,0.0036540285,0.00075256964,0.00039251716,0.0005135597,0.00036577412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021229035,0.00062935986,0.00075464905,0.00093326526,0.00061641674,0.0017427638,0.0011172934,0.0010023491,0.0017354682],"category_scores_gemma":[0.012603271,0.00057295954,0.00030347527,0.00050076406,0.0006466053,0.0012811646,0.0017916416,0.001097206,0.00047026665],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003784387,0.0006206518,0.04797598,0.0004727264,0.00022909718,0.0007992396,0.0005910277,0.25383738,0.19790888,0.113037236,0.006034709,0.37470868],"study_design_scores_gemma":[0.00019063723,0.00018731208,0.0044380724,0.00001954612,0.000038958202,0.00016478574,0.0000363558,0.9395418,0.023607181,0.030525643,0.0012076655,0.0000420821],"about_ca_topic_score_codex":0.0011275853,"about_ca_topic_score_gemma":0.0020957352,"teacher_disagreement_score":0.0021229035,"about_ca_system_score_codex":0.0005019801,"about_ca_system_score_gemma":0.0012380659,"threshold_uncertainty_score":0.011227131},"labels":[],"label_agreement":null},{"id":"W2138703812","doi":"10.1086/382272","title":"A Preliminary Seismic Analysis of 51 Pegasi: Large and Small Spacings from Standard Models","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Range (aeronautics); Metallicity; Astrophysics; Diagram; Space (punctuation); Helium; Star (game theory); Stars; Statistics; Computer science; Mathematics; Atomic physics","score_opus":0.011173485173672993,"score_gpt":0.21445587768858565,"score_spread":0.20328239251491265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138703812","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94314986,0.00011487477,0.043629054,0.00022891375,0.000009491278,0.0000396061,0.000823026,0.00021735214,0.011787888],"genre_scores_gemma":[0.9859239,0.00009452347,0.011538142,0.00001720916,0.00000973068,0.000023761258,0.0012319869,0.000052794538,0.001108006],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980336,0.000046186295,0.000014353383,0.0000447661,0.00006174318,0.000029614785],"domain_scores_gemma":[0.9991947,0.0004137926,0.00009045532,0.00013539616,0.00011013783,0.000055497727],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060509535,0.00033969892,0.000313658,0.0010381453,0.00056710024,0.00079344097,0.00067438104,0.00032169317,0.004582372],"category_scores_gemma":[0.0033071437,0.0002051512,0.00054469175,0.00085277186,0.00038009847,0.000573849,0.00073169294,0.00055728457,0.00034402424],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056025677,0.00018888491,0.18680881,0.0002203,0.00013860584,0.00089740223,0.0009675357,0.61143506,0.014900326,0.09402886,0.003238616,0.08661536],"study_design_scores_gemma":[0.00004066344,0.00021092365,0.07469294,0.000025133406,0.00005226241,0.0003288795,0.00059238635,0.8886721,0.0032561638,0.025220735,0.0068757455,0.000032020333],"about_ca_topic_score_codex":0.005899704,"about_ca_topic_score_gemma":0.006163355,"teacher_disagreement_score":0.005899704,"about_ca_system_score_codex":0.0009162037,"about_ca_system_score_gemma":0.0004171513,"threshold_uncertainty_score":0.015329599},"labels":[],"label_agreement":null},{"id":"W2138976137","doi":"10.1086/317092","title":"Cooling Sequences and Color‐Magnitude Diagrams for Cool White Dwarfs with Hydrogen Atmospheres","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Astrophysics; Physics; Blue dwarf; Atmosphere (unit); Hydrogen; Black dwarf; Ion; Ionization; Stars; Astronomy; Thermodynamics","score_opus":0.008683034028960987,"score_gpt":0.2164311194268263,"score_spread":0.20774808539786532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2138976137","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.977853,0.00014791139,0.007023195,0.00005065154,0.00000953031,0.000023490813,0.0009064777,0.0005338343,0.013451961],"genre_scores_gemma":[0.9914466,0.000063173735,0.005682213,0.000017568998,0.000009707964,0.000018972753,0.0011795802,0.00007479092,0.0015075252],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996305,0.0000050363233,0.0000020941247,0.000007078647,0.0000061884416,0.000016485963],"domain_scores_gemma":[0.9994893,0.00012699876,0.00012800009,0.000036437108,0.00011622462,0.00010313923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001397513,0.00019287819,0.0000934511,0.0015324835,0.0002001304,0.00031867056,0.00017263262,0.00012250415,0.0030985905],"category_scores_gemma":[0.0005759721,0.000079395955,0.00015620279,0.00027722312,0.00020759807,0.0002343348,0.00025288112,0.00022616336,0.00036052577],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017320025,0.00018405,0.630271,0.00021972177,0.00007732336,0.0006084088,0.0015501993,0.05152507,0.12956902,0.047557246,0.006569475,0.1301365],"study_design_scores_gemma":[0.000074337746,0.00028544004,0.87989646,0.000024807681,0.000046379922,0.00068835943,0.00025002097,0.06751775,0.019919485,0.012085727,0.019171843,0.00003943047],"about_ca_topic_score_codex":0.0025946961,"about_ca_topic_score_gemma":0.0024139015,"teacher_disagreement_score":0.0030985905,"about_ca_system_score_codex":0.00029972434,"about_ca_system_score_gemma":0.00011634391,"threshold_uncertainty_score":0.010365784},"labels":[],"label_agreement":null},{"id":"W2139015756","doi":"10.1088/0004-637x/803/2/79","title":"THE ATACAMA COSMOLOGY TELESCOPE: THE LABOCA/ACT SURVEY OF CLUSTERS AT ALL REDSHIFTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Bolometer; Cosmic microwave background; South Pole Telescope; Spire (mollusc); Redshift; RADIUS; Galaxy; Galaxy cluster; Source counts; Cosmology","score_opus":0.02063066554495378,"score_gpt":0.2452471100874241,"score_spread":0.22461644454247032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139015756","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.39998758,0.0026848281,0.0040512057,0.0036596209,0.00037614407,0.0004845591,0.41973296,0.0021043834,0.1669186],"genre_scores_gemma":[0.59218353,0.0022739875,0.017518437,0.0015598406,0.00062217744,0.0006046512,0.30948478,0.00087381096,0.07487874],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954057,0.000043576325,0.000015190491,0.000107278705,0.00021015632,0.00008327033],"domain_scores_gemma":[0.99797946,0.000078495614,0.00034429677,0.0002889385,0.0005649367,0.00074382004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006856233,0.00029080556,0.00034070938,0.0043023694,0.0012809889,0.0013700965,0.0007018971,0.00038567113,0.008717452],"category_scores_gemma":[0.001407691,0.00023016347,0.00019348381,0.0055145673,0.00032105678,0.0009562515,0.0016953263,0.0006823666,0.0037031039],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039900685,0.0001526308,0.45314008,0.00029865713,0.00016098979,0.00018031067,0.0020436156,0.00044093476,0.007126572,0.008958459,0.42669114,0.10040761],"study_design_scores_gemma":[0.00003575085,0.000019350582,0.7713816,0.000053651285,0.000026645572,0.00007952168,0.0005494892,0.00039940735,0.00051662634,0.00067710783,0.22623913,0.000021542834],"about_ca_topic_score_codex":0.17512651,"about_ca_topic_score_gemma":0.27031398,"teacher_disagreement_score":0.17512651,"about_ca_system_score_codex":0.0011328652,"about_ca_system_score_gemma":0.0028422354,"threshold_uncertainty_score":0.34821427},"labels":[],"label_agreement":null},{"id":"W2139046655","doi":"10.1086/524101","title":"The Thermal Regulation of Gravitational Instabilities in Protoplanetary Disks. IV. Simulations with Envelope Irradiation","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Planet; Radiative transfer; Protoplanetary disk; Irradiation; Accretion (finance); Convection; Astrophysics; Gravitation; Radiative cooling; Flux (metallurgy); RADIUS; Instability; Mechanics; Astronomy; Optics; Chemistry; Nuclear physics","score_opus":0.010992829734228342,"score_gpt":0.2186588591150322,"score_spread":0.20766602938080383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139046655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99243027,0.000099293466,0.0016748161,0.00017282112,0.000019619678,0.000026055706,0.00020934721,0.000071051705,0.0052967374],"genre_scores_gemma":[0.998216,0.000049813945,0.00085631,0.000044434204,0.000007848932,0.000021124017,0.00011814288,0.000025967402,0.00066034123],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999268,0.000016341795,0.0000035517717,0.000010715372,0.000012455276,0.000030162342],"domain_scores_gemma":[0.9997372,0.000102597216,0.000047066373,0.00002395468,0.000032041702,0.00005707319],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020641282,0.00043608242,0.00036978678,0.00028431782,0.00047380757,0.0007148199,0.00073194824,0.0008012746,0.0019319741],"category_scores_gemma":[0.0010892941,0.00027211104,0.00064550806,0.00022077553,0.0008607616,0.00054709666,0.00058651937,0.00061109505,0.00019072222],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021630878,0.00012555302,0.011102088,0.00003868174,0.00004091958,0.00018889148,0.00012432566,0.97827554,0.0059413826,0.0020841095,0.00033735245,0.0015249756],"study_design_scores_gemma":[0.000106518906,0.000064221385,0.00407657,0.000007137493,0.000013006208,0.00002522878,0.000062265746,0.9934576,0.001081044,0.0007781212,0.00031811622,0.000010186487],"about_ca_topic_score_codex":0.012329554,"about_ca_topic_score_gemma":0.004926974,"teacher_disagreement_score":0.012329554,"about_ca_system_score_codex":0.0008140555,"about_ca_system_score_gemma":0.00050841115,"threshold_uncertainty_score":0.02451557},"labels":[],"label_agreement":null},{"id":"W2139219201","doi":"10.1086/308419","title":"Using Laboratory Spectroscopy to Identify Lines in the<i>K</i>‐ and<i>L</i>‐Band Spectrum of Water in a Sunspot","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Spectroscopy; Sunspot; Spectrum (functional analysis); Energy spectrum; Astrophysics; Infrared spectroscopy; Atomic physics; Astronomy; Quantum mechanics","score_opus":0.012758728456966836,"score_gpt":0.2952291819983996,"score_spread":0.28247045354143274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139219201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925383,0.000104095285,0.004560331,0.000028928527,0.0000063650104,0.000011092152,0.00009169747,0.00007331825,0.0025858602],"genre_scores_gemma":[0.9955983,0.00007026338,0.0038590152,0.000015290401,0.000004415128,0.000019054782,0.00010541316,0.000010214349,0.0003181032],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992275,0.000015994961,0.000002737334,0.000025507617,0.000017144745,0.000015803022],"domain_scores_gemma":[0.99987745,0.00003237408,0.000035062258,0.0000125513025,0.000022011527,0.000020548878],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015850452,0.00014217242,0.00012736423,0.00055582606,0.0004231536,0.00030218615,0.00031805472,0.00026268724,0.0013240282],"category_scores_gemma":[0.0002463101,0.000101456986,0.0001439813,0.0004838984,0.0002658805,0.00030899668,0.00028479067,0.00028116044,0.0002158181],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037028117,0.00032374996,0.075490914,0.000103467326,0.000057162702,0.00016631116,0.00034361464,0.0014731578,0.8921238,0.0009417197,0.00047639426,0.02812939],"study_design_scores_gemma":[0.00013057026,0.0013349433,0.4486744,0.000032681062,0.000111691385,0.000807078,0.0011180878,0.019749412,0.52191687,0.0018559102,0.0041885567,0.00007984758],"about_ca_topic_score_codex":0.00092750514,"about_ca_topic_score_gemma":0.0018490911,"teacher_disagreement_score":0.0013240282,"about_ca_system_score_codex":0.0001463841,"about_ca_system_score_gemma":0.00014426427,"threshold_uncertainty_score":0.0044293404},"labels":[],"label_agreement":null},{"id":"W2139278132","doi":"10.1086/518643","title":"Mass and Temperature of the TWA 7 Debris Disk","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Debris disk; James Clerk Maxwell Telescope; RADIUS; Stars; Brown dwarf; Context (archaeology); Astronomy; Star formation; Planetary system; Geology","score_opus":0.00477401516888947,"score_gpt":0.2191622414110095,"score_spread":0.21438822624212003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139278132","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988142,0.0000813907,0.000031494787,0.000013412924,0.000001626201,0.0000016431186,0.0001898935,0.000008471097,0.00085785746],"genre_scores_gemma":[0.99901736,0.000042812415,0.0000737246,0.0000057263696,0.000005594657,0.0000024630665,0.0005717186,0.0000046603254,0.00027594852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998934,0.000004252004,0.0000069995276,0.0000350306,0.0000343932,0.00002579826],"domain_scores_gemma":[0.9996019,0.000045489833,0.00013739505,0.000029294748,0.000090820635,0.00009515616],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012059362,0.00013295938,0.00021638638,0.0008919104,0.0003952382,0.000690785,0.00040997312,0.00031531302,0.0013642814],"category_scores_gemma":[0.0005773657,0.00011535818,0.00018281283,0.00033334963,0.00022025242,0.00034366595,0.00042620726,0.00022173922,0.00072490145],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013477071,0.000049969425,0.94273853,0.00003712343,0.000057868674,0.00036226588,0.00066467625,0.00027147404,0.049329158,0.0002365099,0.0003265859,0.005791154],"study_design_scores_gemma":[0.0000025507748,0.00003680731,0.9969062,0.0000043317295,0.000011120309,0.00023450016,0.0001722818,0.0005508658,0.0015063158,0.000052608357,0.00051835336,0.000003980496],"about_ca_topic_score_codex":0.004110673,"about_ca_topic_score_gemma":0.00424112,"teacher_disagreement_score":0.004110673,"about_ca_system_score_codex":0.0007216409,"about_ca_system_score_gemma":0.00010716894,"threshold_uncertainty_score":0.008173466},"labels":[],"label_agreement":null},{"id":"W2139336715","doi":"10.1088/0004-637x/791/1/47","title":"PROBING THE CRUST OF THE NEUTRON STAR IN EXO 0748-676","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Office of Naval Research; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Advanced Research; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution","keywords":"Neutron star; Astrophysics; Accretion (finance); Physics; Crust; Thermal; Swift; Thermal emission; Astronomy; Geophysics","score_opus":0.011789749658691876,"score_gpt":0.2169810341741792,"score_spread":0.20519128451548732,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139336715","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879866,0.00035423425,0.00091439195,0.00020761952,0.000030008572,0.000017728727,0.0018274657,0.000091929265,0.008569951],"genre_scores_gemma":[0.995155,0.00019987636,0.0008138259,0.0001547977,0.00001305359,0.000014460118,0.0020458468,0.00008058963,0.0015226811],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998808,0.000009915276,0.0000060502007,0.000034405497,0.000031704596,0.000037140027],"domain_scores_gemma":[0.99974555,0.000029935978,0.00005167208,0.000030075107,0.000047873065,0.00009477014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031859553,0.0004141408,0.00068949035,0.00054337125,0.00087344926,0.00082581845,0.00041062437,0.0009230302,0.0039790315],"category_scores_gemma":[0.00048236235,0.0004223943,0.00033167808,0.0005040719,0.00041838188,0.0005451322,0.0016453273,0.0009794198,0.0010009492],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024971005,0.00033072403,0.25106597,0.00022695141,0.0002938816,0.0020474133,0.0010515006,0.0026266049,0.72011864,0.0013440383,0.002194666,0.016202478],"study_design_scores_gemma":[0.00010636383,0.00036965503,0.97384036,0.000042496566,0.000077060606,0.00064064836,0.00079584116,0.0036622102,0.014928472,0.0005858922,0.004921315,0.000029714101],"about_ca_topic_score_codex":0.0064336415,"about_ca_topic_score_gemma":0.014522805,"teacher_disagreement_score":0.0064336415,"about_ca_system_score_codex":0.00049321365,"about_ca_system_score_gemma":0.0003624413,"threshold_uncertainty_score":0.013311148},"labels":[],"label_agreement":null},{"id":"W2139358959","doi":"10.1088/0004-637x/794/2/127","title":"INDUCED CORE FORMATION TIME IN SUBCRITICAL MAGNETIC CLOUDS BY LARGE-SCALE TRANS-ALFVÉNIC FLOWS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Scale (ratio); Core (optical fiber); Physics; Mechanics; Atmospheric sciences; Geology; Environmental science; Optics","score_opus":0.008474105113476653,"score_gpt":0.22844122273262843,"score_spread":0.21996711761915178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139358959","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9934129,0.0000447173,0.0049191713,0.000037025944,0.000008014901,0.000009425371,0.000016251232,0.00004589117,0.0015066147],"genre_scores_gemma":[0.99914455,0.000016679774,0.00070684426,0.0000056777358,0.0000014074305,0.0000053745416,0.000010378836,0.0000053645667,0.00010365991],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996185,0.000005808863,0.0000018262054,0.0000049221476,0.000008184938,0.00001739422],"domain_scores_gemma":[0.9997694,0.00006834779,0.00006796125,0.00002240684,0.000027748663,0.00004413029],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014175332,0.00015040812,0.00018402585,0.00020294303,0.00037170883,0.00028197735,0.00028245142,0.0001693975,0.0005344478],"category_scores_gemma":[0.00062691583,0.00011338651,0.0002959255,0.00010581755,0.00036086602,0.00029198907,0.00031219202,0.00030724177,0.000044779823],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041191195,0.00021609056,0.017838378,0.00009974851,0.000083025516,0.0007342529,0.0004903383,0.7822336,0.16306758,0.025744561,0.00054609764,0.008534371],"study_design_scores_gemma":[0.000053539752,0.000068896574,0.0052334806,0.0000045539564,0.000011119883,0.000042721527,0.000028493163,0.97296244,0.019229315,0.0020577165,0.00029537937,0.000012361572],"about_ca_topic_score_codex":0.0038326092,"about_ca_topic_score_gemma":0.0017133558,"teacher_disagreement_score":0.0038326092,"about_ca_system_score_codex":0.0006180327,"about_ca_system_score_gemma":0.0004242346,"threshold_uncertainty_score":0.007620573},"labels":[],"label_agreement":null},{"id":"W2139370468","doi":"10.1086/587685","title":"Structural Analysis of Molecular Clouds: Dendrograms","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":574,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Dendrogram; Isosurface; Data cube; Data set; Line (geometry); Pattern recognition (psychology); Range (aeronautics); Data point; Interpolation (computer graphics)","score_opus":0.011359693054295605,"score_gpt":0.2406832506483921,"score_spread":0.2293235575940965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139370468","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.35820892,0.001324533,0.61137426,0.0012515837,0.000113062386,0.00045690982,0.010567297,0.0070818383,0.009621596],"genre_scores_gemma":[0.7107215,0.00075606816,0.27716702,0.000090676665,0.000063571664,0.00026994443,0.008689085,0.00078710285,0.0014551],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994332,0.00012409117,0.000048442293,0.00012595723,0.00019212157,0.000075983415],"domain_scores_gemma":[0.996678,0.0012473018,0.0005475255,0.00043729955,0.00087607367,0.00021383923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009823004,0.00042733987,0.0004945523,0.008660027,0.0010721356,0.0026340995,0.0008627845,0.0005159697,0.002961077],"category_scores_gemma":[0.005895798,0.00035188012,0.0007428263,0.0068268087,0.0007499283,0.0020186335,0.0014465606,0.00089462375,0.0007825322],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007304965,0.00030455514,0.1264152,0.0012351541,0.00052588497,0.0012902264,0.006937132,0.25182188,0.04480172,0.16036077,0.024341432,0.38123554],"study_design_scores_gemma":[0.000043411743,0.00008197786,0.047171295,0.00020249971,0.00009143477,0.0004728583,0.0022062783,0.7797916,0.008468327,0.12700719,0.03432967,0.0001335854],"about_ca_topic_score_codex":0.007334791,"about_ca_topic_score_gemma":0.005765577,"teacher_disagreement_score":0.008660027,"about_ca_system_score_codex":0.0011812358,"about_ca_system_score_gemma":0.0009315486,"threshold_uncertainty_score":0.014584184},"labels":[],"label_agreement":null},{"id":"W2139445185","doi":"10.1086/431642","title":"Hα‐derived Star Formation Rates for Three<i>z</i>≃0.75 EDisCS Galaxy Clusters","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":160,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Galaxy; Star formation; Redshift; Cluster (spacecraft); Galaxy cluster; Stellar mass; Brightest cluster galaxy; Star cluster; Astronomy","score_opus":0.00960398245888911,"score_gpt":0.2305488458246883,"score_spread":0.2209448633657992,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139445185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950513,0.00007779544,0.00014239796,0.00002472578,0.000005266436,0.000008610607,0.0024599864,0.000061833576,0.0021680968],"genre_scores_gemma":[0.9917874,0.00005530613,0.00039238628,0.000022093915,0.000008652414,0.000007108599,0.006369708,0.000022777822,0.001334689],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986136,0.000007551952,0.000008895524,0.000048779093,0.000026986816,0.00004643365],"domain_scores_gemma":[0.9984723,0.0001996313,0.00026362692,0.00018439509,0.0003982417,0.00048176496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046099946,0.0003039655,0.00031664514,0.001356274,0.0005842962,0.0005796482,0.0006276686,0.00026587743,0.002921352],"category_scores_gemma":[0.0010310162,0.0002612247,0.00032293025,0.0006344812,0.00038242768,0.00020865617,0.00064980565,0.00019520473,0.0009906669],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010644329,0.00005294231,0.9627019,0.000090412796,0.000114988135,0.00011904343,0.00049495604,0.003460269,0.013303344,0.00091837335,0.0061859335,0.011493361],"study_design_scores_gemma":[0.000016416907,0.000018369097,0.9957365,0.000004125272,0.000023366978,0.00003767369,0.00009753536,0.0011042428,0.0021184473,0.00009265965,0.0007416488,0.000008951069],"about_ca_topic_score_codex":0.02367488,"about_ca_topic_score_gemma":0.039813813,"teacher_disagreement_score":0.02367488,"about_ca_system_score_codex":0.00082749623,"about_ca_system_score_gemma":0.00030137738,"threshold_uncertainty_score":0.04707414},"labels":[],"label_agreement":null},{"id":"W2139668579","doi":"10.1086/518028","title":"VLBA Measurement of the Transverse Velocity of the Magnetar XTE J1810−197","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Magnetar; Physics; Neutron star; Astrophysics; Proper motion; Very Long Baseline Array; Telescope; Radio telescope; Position angle; Transverse plane; Astronomy; Stars; Biology; Galaxy; Quasar","score_opus":0.016834706655515563,"score_gpt":0.28389001865908664,"score_spread":0.2670553120035711,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139668579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970055,0.00006670356,0.0005557609,0.000031348656,0.000008968205,0.0000041636995,0.00042418393,0.000027985781,0.001875545],"genre_scores_gemma":[0.99656147,0.0000867339,0.0011126895,0.000028696255,0.000018675395,0.000008514717,0.00131572,0.00001143982,0.0008560594],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998926,0.000012796425,0.000005923062,0.000032322587,0.000025453875,0.000030779047],"domain_scores_gemma":[0.99967325,0.000033607,0.000114069386,0.00004383906,0.00006548398,0.00006980027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002105415,0.0001469924,0.00016159941,0.00061895605,0.00027216008,0.0005263928,0.00027334745,0.00018322309,0.0009309696],"category_scores_gemma":[0.00047701667,0.00015932246,0.00010111528,0.000502805,0.00020591,0.00023606897,0.00026394427,0.00027703764,0.00042075268],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044996152,0.00017288368,0.75626916,0.000043474374,0.00009545177,0.00043073593,0.00036511346,0.0008940957,0.22288556,0.0009073454,0.00069479906,0.016791424],"study_design_scores_gemma":[0.000033649765,0.0001847443,0.9768759,0.000013913582,0.000044294804,0.0004800452,0.00013423705,0.0018008538,0.017526057,0.00011158303,0.0027805546,0.000014088483],"about_ca_topic_score_codex":0.0040640496,"about_ca_topic_score_gemma":0.0094300965,"teacher_disagreement_score":0.0040640496,"about_ca_system_score_codex":0.00039459593,"about_ca_system_score_gemma":0.00020980027,"threshold_uncertainty_score":0.0080807805},"labels":[],"label_agreement":null},{"id":"W2139773694","doi":"10.1086/339210","title":"Optical Identification of Multiple Faint X‐Ray Sources in the Globular Cluster NGC 6752: Evidence for Numerous Cataclysmic Variables1","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Globular cluster; Millisecond pulsar; Luminosity; Hubble space telescope; RADIUS; Advanced Camera for Surveys; Cluster (spacecraft); Star cluster","score_opus":0.03393340214880842,"score_gpt":0.26069950521241164,"score_spread":0.22676610306360323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139773694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992518,0.00023255506,0.00010442547,0.000017964989,0.000003460757,0.0000033012006,0.000053148055,0.000006842276,0.00032649195],"genre_scores_gemma":[0.9992174,0.00009192841,0.000313857,0.000021613194,0.000014936353,0.0000030432798,0.0002099736,0.0000020162752,0.00012515995],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997439,0.000023764025,0.00002041416,0.000058212125,0.00006904158,0.000084790685],"domain_scores_gemma":[0.99884975,0.00015873314,0.00048883783,0.00012020192,0.0001248375,0.00025770903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033502706,0.00039839212,0.00020563298,0.0017087953,0.0008049012,0.0008872219,0.00049826223,0.00041308746,0.0011919201],"category_scores_gemma":[0.0007849879,0.00027676282,0.00014032575,0.0010171172,0.0007034641,0.00037647222,0.00088625745,0.00024442314,0.00031204708],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000113980794,0.000054399166,0.98047936,0.000032818734,0.00003253568,0.000771864,0.00036783298,0.00009640841,0.009806813,0.00020758843,0.0002797497,0.0077566984],"study_design_scores_gemma":[0.000011016443,0.000075289325,0.9964881,0.00000958989,0.000027280628,0.001663416,0.00016235454,0.0001651886,0.00076488714,0.00008527827,0.000539419,0.000008255121],"about_ca_topic_score_codex":0.008331814,"about_ca_topic_score_gemma":0.019014763,"teacher_disagreement_score":0.008331814,"about_ca_system_score_codex":0.0002914195,"about_ca_system_score_gemma":0.0002480368,"threshold_uncertainty_score":0.016566634},"labels":[],"label_agreement":null},{"id":"W2139796538","doi":"10.1088/0004-637x/760/2/130","title":"THE PROPERTIES OF THE STAR-FORMING INTERSTELLAR MEDIUM AT<i>z</i>= 0.8–2.2 FROM HiZELS: STAR FORMATION AND CLUMP SCALING LAWS IN GAS-RICH, TURBULENT DISKS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":158,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Interstellar medium; Galaxy; Velocity dispersion; Molecular cloud; Scaling; Star (game theory); Spectroscopy; Stars; Astronomy","score_opus":0.016276568046999368,"score_gpt":0.2187057429861664,"score_spread":0.20242917493916704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139796538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99948895,0.000053106447,0.00008438746,0.0000067522938,5.3172886e-7,0.0000014334406,0.000068051595,0.00000796999,0.00028895226],"genre_scores_gemma":[0.999559,0.00002489048,0.00012241816,0.000004416249,0.0000022016807,0.0000012712635,0.00022042607,0.0000017759226,0.00006367266],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999603,0.0000024712622,0.0000021818505,0.000009328767,0.00000952299,0.000016234446],"domain_scores_gemma":[0.9998387,0.000017237799,0.00006817058,0.000010292042,0.00001926461,0.000046292396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008249519,0.00016818127,0.00012931514,0.00078787236,0.0002810696,0.0005368819,0.00023408871,0.00014843809,0.00058231805],"category_scores_gemma":[0.00023830596,0.00014081567,0.00009740756,0.00039030757,0.00019188305,0.0002688299,0.00034645817,0.00014091184,0.00016750989],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014871501,0.000035672885,0.9431607,0.0000149626685,0.00003413673,0.00028779436,0.000290361,0.00056274614,0.049534805,0.00021138258,0.00021537911,0.0055032037],"study_design_scores_gemma":[0.0000034077332,0.000017422113,0.997166,0.0000012107306,0.000008025342,0.00014186835,0.000099359844,0.00075378205,0.00152847,0.000052804902,0.00022506093,0.0000026449882],"about_ca_topic_score_codex":0.004552668,"about_ca_topic_score_gemma":0.007061084,"teacher_disagreement_score":0.004552668,"about_ca_system_score_codex":0.00025935253,"about_ca_system_score_gemma":0.00006808844,"threshold_uncertainty_score":0.009052336},"labels":[],"label_agreement":null},{"id":"W2139842428","doi":"10.1086/421259","title":"X‐Ray Sources and Their Optical Counterparts in the Globular Cluster M4","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Globular cluster; ROSAT; Hubble space telescope; Millisecond pulsar; Luminosity; Astrometry; Cluster (spacecraft); Observatory; Open cluster","score_opus":0.008604796508327898,"score_gpt":0.21523860482242943,"score_spread":0.20663380831410152,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139842428","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997493,0.00020829326,0.00010543122,0.00003431656,0.0000023668308,0.000004402626,0.00019212256,0.000009613505,0.0019505364],"genre_scores_gemma":[0.9975636,0.00018104378,0.00054794824,0.000025904343,0.000016500386,0.000008713686,0.00068072206,0.0000047835206,0.00097074144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998549,0.000012528704,0.000009107145,0.000025108253,0.000038688595,0.000059654707],"domain_scores_gemma":[0.9995704,0.00005570114,0.00021108013,0.00004043315,0.000050828803,0.00007147968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015460746,0.00026193846,0.00020941775,0.0023610229,0.0009666875,0.0006743852,0.00034476657,0.00037908775,0.002547234],"category_scores_gemma":[0.000674417,0.00023538525,0.00021014763,0.0015493673,0.00043574083,0.00045113923,0.0009960158,0.00018122359,0.00046124603],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004999642,0.00007756417,0.9707051,0.00004286516,0.000038027163,0.0008236102,0.0005219267,0.0003659807,0.012744584,0.00073726755,0.00039415472,0.0130490335],"study_design_scores_gemma":[0.000026140217,0.00009739399,0.99349135,0.000015041615,0.000036355526,0.0012899064,0.0002689719,0.0003096849,0.0014376155,0.0006240475,0.0023929942,0.000010616072],"about_ca_topic_score_codex":0.009064181,"about_ca_topic_score_gemma":0.009718288,"teacher_disagreement_score":0.009064181,"about_ca_system_score_codex":0.0006447914,"about_ca_system_score_gemma":0.00034310055,"threshold_uncertainty_score":0.018022835},"labels":[],"label_agreement":null},{"id":"W2139974220","doi":"10.1086/383534","title":"High‐Energy Gamma‐Ray Observations of W Comae with the Solar Tower Atmospheric Cerenkov Effect Experiment (STACEE)","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; TRIUMF; McGill University","funders":"","keywords":"Physics; Hadron; Context (archaeology); Tower; Jet (fluid); Astrophysics; Blazar; Nuclear physics; Gamma ray","score_opus":0.006060697581810772,"score_gpt":0.1977150675007607,"score_spread":0.19165436991894994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2139974220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957424,0.00006167898,0.0005195826,0.00003739828,0.000003661606,0.000014153193,0.00037637202,0.000029465904,0.0032153146],"genre_scores_gemma":[0.9968514,0.00011087173,0.0012018137,0.00002213547,0.000010910095,0.0000056202734,0.0011982166,0.000008990434,0.00058996596],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982387,0.000035325924,0.0000055832998,0.000026261916,0.00006459479,0.0000444039],"domain_scores_gemma":[0.9992625,0.00011012955,0.00025280818,0.00013967934,0.00008895781,0.00014591604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054650276,0.0003303051,0.00018232019,0.00064098404,0.0006025316,0.00041969612,0.00026860138,0.00017758166,0.0008838906],"category_scores_gemma":[0.00078747456,0.00018817402,0.00025997244,0.0006857184,0.00033761325,0.00023520981,0.0005095901,0.00028429125,0.00018700531],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046121102,0.00015871451,0.9594821,0.000045069704,0.00016346882,0.00039372835,0.00046660024,0.0012072736,0.020496773,0.0009819417,0.0013045842,0.014838583],"study_design_scores_gemma":[0.000029160476,0.00020435516,0.99030674,0.000006108819,0.00003131528,0.00028351837,0.000094619616,0.0014592451,0.0029629038,0.00031534064,0.004295942,0.000010759064],"about_ca_topic_score_codex":0.008646835,"about_ca_topic_score_gemma":0.04090349,"teacher_disagreement_score":0.008646835,"about_ca_system_score_codex":0.00034082684,"about_ca_system_score_gemma":0.00024693485,"threshold_uncertainty_score":0.01719302},"labels":[],"label_agreement":null},{"id":"W2140096485","doi":"10.1088/0004-637x/699/2/l134","title":"THE PERILS OF CLUMPFIND: THE MASS SPECTRUM OF SUBSTRUCTURES IN MOLECULAR CLOUDS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Mass spectrum; Astrophysics; Molecular cloud; Physics; Emission spectrum; Dimension (graph theory); Robustness (evolution); Spectrum (functional analysis); Function (biology); Line (geometry); Spectral line; Mass spectrometry; Astronomy; Chemistry; Mathematics; Geometry; Quantum mechanics; Combinatorics","score_opus":0.004458812011527593,"score_gpt":0.2245183414564797,"score_spread":0.2200595294449521,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140096485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99642426,0.0001077194,0.0025644007,0.00007022563,0.0000059589797,0.000006599425,0.00015377281,0.00011449689,0.0005524896],"genre_scores_gemma":[0.996774,0.00003002094,0.0027257309,0.000018776629,0.000009797656,0.000004707346,0.0002967225,0.000048348335,0.00009194804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997842,0.000041579377,0.00000821976,0.00006186276,0.000074564254,0.000029515362],"domain_scores_gemma":[0.9982071,0.0009017824,0.00035504205,0.0002619207,0.0001251933,0.00014890725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00091844815,0.00030373258,0.00015247132,0.0011721915,0.00026160976,0.0009140287,0.00060454605,0.0005558602,0.00040553857],"category_scores_gemma":[0.003547405,0.00017595853,0.00040890253,0.000589286,0.00060947245,0.00064384117,0.0007117453,0.00048339847,0.00010335037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015609849,0.00035752277,0.63298446,0.00018805123,0.00042697747,0.001739193,0.0012930897,0.20381111,0.0836037,0.0069383685,0.0017371466,0.06535944],"study_design_scores_gemma":[0.000071737515,0.0001729947,0.4598035,0.00004257382,0.000051438186,0.00047208683,0.00033485628,0.51206005,0.021977743,0.0037052261,0.0012473812,0.000060349274],"about_ca_topic_score_codex":0.0031576427,"about_ca_topic_score_gemma":0.0025883252,"teacher_disagreement_score":0.0031576427,"about_ca_system_score_codex":0.0005360679,"about_ca_system_score_gemma":0.00017767379,"threshold_uncertainty_score":0.006278515},"labels":[],"label_agreement":null},{"id":"W2140097971","doi":"10.1086/431922","title":"<i>FUSE</i>Measurements of Far‐Ultraviolet Extinction. II. Magellanic Cloud Sight Lines","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Milky Way; Extinction (optical mineralogy); Astrophysics; Small Magellanic Cloud; Large Magellanic Cloud; Wavelength; Astronomy; Line-of-sight; Ultraviolet; Galaxy; Optics","score_opus":0.01759789013921602,"score_gpt":0.2431209692112948,"score_spread":0.2255230790720788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140097971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9751219,0.00074880815,0.0031106514,0.000040324096,0.000009854327,0.000010549226,0.008416114,0.00031127746,0.012230615],"genre_scores_gemma":[0.9905117,0.0002413081,0.0028584981,0.00003610411,0.000013251798,0.000007429701,0.005605402,0.000030420284,0.0006959741],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999372,0.000003600396,0.000003313429,0.00001457582,0.000022485743,0.000018822513],"domain_scores_gemma":[0.9997284,0.00003478594,0.00012248037,0.00002794777,0.000048301205,0.000038035505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011256313,0.00022497681,0.00007643027,0.002080136,0.00025109123,0.00024850477,0.00018938558,0.00019740681,0.0014165215],"category_scores_gemma":[0.00025438427,0.000064854954,0.00020215489,0.0007588179,0.000096614946,0.00028260148,0.00020133198,0.0001793367,0.0003289466],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001615163,0.000043132317,0.884063,0.000066017405,0.000110826695,0.00019783108,0.00021067305,0.0021979772,0.07739725,0.00086531194,0.0032218483,0.031464677],"study_design_scores_gemma":[0.0000015074903,0.00002431753,0.98729116,0.000006678118,0.000017978498,0.00014168561,0.0000384253,0.001032862,0.008669869,0.00011957266,0.0026498507,0.0000060888287],"about_ca_topic_score_codex":0.009698578,"about_ca_topic_score_gemma":0.01276439,"teacher_disagreement_score":0.009698578,"about_ca_system_score_codex":0.0004154922,"about_ca_system_score_gemma":0.000091033886,"threshold_uncertainty_score":0.019284248},"labels":[],"label_agreement":null},{"id":"W2140131843","doi":"10.1088/0004-637x/716/1/819","title":"VERITAS 2008-2009 MONITORING OF THE VARIABLE GAMMA-RAY SOURCE M 87","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Flare; Crab Nebula; Astrophysics; Flux (metallurgy); Astronomy; Gamma ray; Radio galaxy; Observatory; Spectral index; Blazar; Wavelength; Galaxy; Spectral line; Optics","score_opus":0.005383396390725562,"score_gpt":0.20341139731185826,"score_spread":0.1980280009211327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140131843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956793,0.00010412817,0.00030947133,0.000046721132,0.000009283737,0.00001969882,0.0015142781,0.00013397267,0.0021831105],"genre_scores_gemma":[0.9914426,0.00009762484,0.0018329963,0.00006331232,0.000023729535,0.000021350605,0.00507332,0.000030701387,0.0014143449],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997936,0.000010709398,0.000008548778,0.000058496677,0.00008311811,0.00004555526],"domain_scores_gemma":[0.9995726,0.000029056995,0.00015607689,0.000054288204,0.00011848884,0.000069591595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002559725,0.00017896805,0.00022954281,0.0008087711,0.0002590572,0.00033791692,0.0004799917,0.00022842782,0.00079605874],"category_scores_gemma":[0.0005520173,0.00014009941,0.00017823953,0.00038670044,0.00015199634,0.00020360782,0.0006275953,0.00038133463,0.00024703424],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001220548,0.00024515454,0.779346,0.00016053068,0.00019141278,0.0011132299,0.0013371045,0.0020616027,0.12829374,0.0007200334,0.0090358555,0.0762748],"study_design_scores_gemma":[0.000029147519,0.00013805674,0.98709434,0.000014494124,0.000032512064,0.0003258304,0.000119301905,0.001802248,0.0058395364,0.000038029313,0.0045551667,0.000011288034],"about_ca_topic_score_codex":0.015575647,"about_ca_topic_score_gemma":0.04186065,"teacher_disagreement_score":0.015575647,"about_ca_system_score_codex":0.0007260467,"about_ca_system_score_gemma":0.0003281585,"threshold_uncertainty_score":0.030969977},"labels":[],"label_agreement":null},{"id":"W2140328825","doi":"10.1088/0004-637x/772/1/50","title":"TIMING AND INTERSTELLAR SCATTERING OF 35 DISTANT PULSARS DISCOVERED IN THE PALFA SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Physics; Astrophysics; Astronomy; Glitch; Observatory; Interstellar medium; Population; Nebula; Scattering; Line-of-sight; Stars; Galaxy","score_opus":0.021145367997361247,"score_gpt":0.30554124976466374,"score_spread":0.28439588176730246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140328825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99800867,0.00006662875,0.00009469441,0.00002268837,0.0000022945121,0.0000053273097,0.0005547342,0.0000117222335,0.0012332624],"genre_scores_gemma":[0.9969195,0.00008326245,0.00034719944,0.00002039403,0.000012024608,0.000007970749,0.0019575916,0.000006193269,0.000645862],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984014,0.000020431611,0.0000070120964,0.000052257354,0.00004356055,0.000036588724],"domain_scores_gemma":[0.9992894,0.000097487726,0.0002296771,0.00007838889,0.0001359094,0.00016915653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028992386,0.00019991986,0.00019745274,0.0012906712,0.00031169236,0.00040482346,0.00022915575,0.0001455644,0.001025652],"category_scores_gemma":[0.0006865073,0.00012103566,0.00015434423,0.0006905467,0.00023787828,0.0001940314,0.0005725651,0.0002488932,0.00026619577],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001949536,0.000055432578,0.96981436,0.00002986655,0.000062475614,0.0005061505,0.00086659426,0.00023680221,0.012272023,0.00015838101,0.0005956535,0.015207275],"study_design_scores_gemma":[0.0000039010697,0.000023104933,0.9986356,0.0000020039893,0.0000053998433,0.00013628058,0.0000828634,0.00008619602,0.00019723206,0.000011620472,0.00081330416,0.00000242259],"about_ca_topic_score_codex":0.010315419,"about_ca_topic_score_gemma":0.022807954,"teacher_disagreement_score":0.010315419,"about_ca_system_score_codex":0.00038138172,"about_ca_system_score_gemma":0.0001503578,"threshold_uncertainty_score":0.020510733},"labels":[],"label_agreement":null},{"id":"W2140442400","doi":"10.1086/422987","title":"Radiative Transfer and Starless Cores","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Opacity; Radiative transfer; Molecular cloud; Line (geometry); Millimeter; Hyperfine structure; Spectral line; Lambda","score_opus":0.009117665031679276,"score_gpt":0.22801724614806512,"score_spread":0.21889958111638586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140442400","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.27865258,0.00020036788,0.71572,0.00008805855,0.00001610885,0.00005118191,0.0000786855,0.0004720698,0.004720941],"genre_scores_gemma":[0.89736754,0.00006201754,0.100690335,0.000026262083,0.000019753908,0.000042168285,0.0000840874,0.00006723023,0.0016405563],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998091,0.000052728097,0.000005022445,0.000041670486,0.00007155691,0.000019992056],"domain_scores_gemma":[0.9993131,0.0003037688,0.00014322731,0.00011240914,0.00008733336,0.00004021802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038212648,0.00023419967,0.00019802875,0.0003529068,0.00025830843,0.00048276552,0.00090506225,0.0002855201,0.001194335],"category_scores_gemma":[0.002655362,0.00021065677,0.0003108881,0.00030781113,0.000578488,0.0007409973,0.00061398925,0.00040023166,0.00020482636],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020057768,0.00017236068,0.034034576,0.00014589344,0.00009921961,0.00040878763,0.00082833157,0.58345455,0.04503749,0.17499885,0.0013488441,0.15927052],"study_design_scores_gemma":[0.000032501855,0.000056374683,0.0049633672,0.000005961771,0.000007875364,0.00015703784,0.000040098737,0.9234659,0.009544722,0.059642583,0.0020691901,0.0000144134665],"about_ca_topic_score_codex":0.0016987564,"about_ca_topic_score_gemma":0.0015766901,"teacher_disagreement_score":0.0016987564,"about_ca_system_score_codex":0.00036733417,"about_ca_system_score_gemma":0.00035370927,"threshold_uncertainty_score":0.0039954185},"labels":[],"label_agreement":null},{"id":"W2140620106","doi":"10.1086/421105","title":"Extended Mosaic Observations with the Cosmic Background Imager","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":330,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Mosaic; COSMIC cancer database; Sky; Cosmology; Universe","score_opus":0.014368419389060022,"score_gpt":0.2470778461342665,"score_spread":0.23270942674520648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140620106","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9245471,0.001518494,0.009816545,0.00035335447,0.000100879086,0.00009885925,0.009909467,0.001792005,0.051863376],"genre_scores_gemma":[0.970731,0.00036737582,0.017159348,0.000102234735,0.00010378213,0.000028942482,0.00856926,0.0002057092,0.0027322269],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967027,0.000028899707,0.0000069050284,0.00009298749,0.00013717938,0.00006372434],"domain_scores_gemma":[0.9996371,0.000014549507,0.000058439797,0.00009636114,0.00009717749,0.00009648316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036520825,0.00017227481,0.0002536802,0.0011279634,0.00034557542,0.0006180792,0.00020776162,0.00022784791,0.0016683476],"category_scores_gemma":[0.0004715698,0.00018131934,0.00029684982,0.0013532373,0.00015205434,0.0004062916,0.0006133716,0.00033640748,0.00046503125],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015478375,0.00046974537,0.42226642,0.00020347648,0.00089154503,0.0006734653,0.00092152663,0.0066279694,0.3287047,0.009418461,0.029950388,0.19832446],"study_design_scores_gemma":[0.00008008674,0.00009769192,0.96112263,0.00002598417,0.00011630779,0.00024634623,0.00009762188,0.0061509283,0.004945385,0.0013938965,0.025696479,0.000026634587],"about_ca_topic_score_codex":0.014887904,"about_ca_topic_score_gemma":0.034099035,"teacher_disagreement_score":0.014887904,"about_ca_system_score_codex":0.00040264602,"about_ca_system_score_gemma":0.00054606335,"threshold_uncertainty_score":0.029602468},"labels":[],"label_agreement":null},{"id":"W2140688245","doi":"10.1086/386536","title":"First Year<i>Wilkinson Microwave Anisotropy Probe</i>Observations: Dark Energy Induced Correlation with Radio Sources","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":206,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"CMB cold spot; Physics; Cosmic microwave background; Astrophysics; Dark energy; Omega; Planck; Cosmology; Lambda; Spectral density; Dark matter; Universe; Anisotropy; Quantum mechanics; Statistics","score_opus":0.008843868539942023,"score_gpt":0.20610368134548307,"score_spread":0.19725981280554106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2140688245","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98375976,0.00032968086,0.0045182393,0.00020808878,0.000031913703,0.00001665435,0.0023490142,0.0002786783,0.00850796],"genre_scores_gemma":[0.9963821,0.00009041481,0.0012046465,0.00007135736,0.000039113733,0.000010965214,0.0013000644,0.000026236437,0.00087519916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997117,0.000035162386,0.000015675283,0.00007313774,0.000090199086,0.00007403875],"domain_scores_gemma":[0.99708277,0.000636017,0.0011647086,0.0005391606,0.00021213581,0.00036510255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005265233,0.00031039765,0.00020748586,0.0020871556,0.0003189505,0.001182348,0.00042926677,0.0002898603,0.003020309],"category_scores_gemma":[0.0023841066,0.00012549896,0.0002593753,0.0017839576,0.00040693252,0.00050230225,0.0006574562,0.00046728656,0.0004963211],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034467294,0.000049901704,0.9325927,0.00007430115,0.00017727885,0.000658095,0.00035545893,0.0015449704,0.031643298,0.0051861415,0.0041529313,0.023220353],"study_design_scores_gemma":[0.000009418917,0.000048700454,0.98125684,0.000010491921,0.000037585916,0.0004677975,0.00008382966,0.0020305794,0.010784923,0.0012202966,0.004027548,0.000021892165],"about_ca_topic_score_codex":0.002301336,"about_ca_topic_score_gemma":0.0033257187,"teacher_disagreement_score":0.003020309,"about_ca_system_score_codex":0.00031516847,"about_ca_system_score_gemma":0.00013890289,"threshold_uncertainty_score":0.010103941},"labels":[],"label_agreement":null},{"id":"W2141067605","doi":"10.1088/0004-637x/721/1/777","title":"CORE-COLLAPSE SUPERNOVAE FROM THE PALOMAR TRANSIENT FACTORY: INDICATIONS FOR A DIFFERENT POPULATION IN DWARF GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":207,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Supernova; Transient (computer programming); Astrophysics; Galaxy; Physics; Dwarf galaxy; Factory (object-oriented programming); Globular cluster; Astronomy; Population; Computer science; Medicine","score_opus":0.02167676887662592,"score_gpt":0.25196186296306006,"score_spread":0.23028509408643413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141067605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99835014,0.000098725155,0.00018437007,0.000008973948,0.0000014752727,0.0000056349536,0.00093297614,0.000023026254,0.0003947291],"genre_scores_gemma":[0.99511236,0.00009387307,0.00027282164,0.000019783836,0.0000057357383,0.000008336653,0.004282243,0.000010581883,0.00019435766],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999798,0.000019139321,0.000017084618,0.00007501434,0.000039416846,0.00005136574],"domain_scores_gemma":[0.99878496,0.00015800002,0.00041079428,0.00019612724,0.00012249673,0.00032758262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040106595,0.00029998878,0.00037294548,0.0026285043,0.00029734094,0.0007909302,0.00027701413,0.0001842636,0.0012567724],"category_scores_gemma":[0.00078848185,0.0001507707,0.0003087028,0.00108199,0.00027362147,0.00037341542,0.00081701676,0.00018063394,0.0004279634],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005882531,0.000013626863,0.9950749,0.00000930875,0.000027435552,0.00011766067,0.00012321609,0.00003680906,0.0018203986,0.000026355843,0.00008831727,0.0026030971],"study_design_scores_gemma":[0.0000028655763,0.000022683682,0.9991441,0.000002187227,0.0000069567895,0.00027891016,0.00008241612,0.00007876264,0.00015409934,0.0000132477135,0.0002121343,0.0000017139785],"about_ca_topic_score_codex":0.0063978676,"about_ca_topic_score_gemma":0.0073580025,"teacher_disagreement_score":0.0063978676,"about_ca_system_score_codex":0.00025626528,"about_ca_system_score_gemma":0.00020289177,"threshold_uncertainty_score":0.0127212405},"labels":[],"label_agreement":null},{"id":"W2141145035","doi":"10.1088/0004-637x/746/2/151","title":"THE 2010 VERY HIGH ENERGY γ-RAY FLARE AND 10 YEARS OF MULTI-WAVELENGTH OBSERVATIONS OF M 87","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Japan Aerospace Exploration Agency; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Istituto Nazionale di Fisica Nucleare; Natural Sciences and Engineering Research Council of Canada; Istituto Nazionale di Astrofisica; Univerzita Karlova v Praze; Centre National de la Recherche Scientifique; Smithsonian Institution; U.S. Department of Energy; National Radio Astronomy Observatory; Vetenskapsrådet; Max-Planck-Gesellschaft; National Research Foundation; High Energy Accelerator Research Organization; Ministerio de Ciencia e Innovación; Bundesministerium für Bildung und Forschung; Office of Science; Academy of Finland; University of Namibia; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Ministry of Education, Culture, Sports, Science and Technology; Deutsche Forschungsgemeinschaft; Agenzia Spaziale Italiana; Helmholtz-Gemeinschaft; National Aeronautics and Space Administration; Associated Universities; Science Foundation Ireland; National Science Foundation","keywords":"Physics; Flare; Astrophysics; Supermassive black hole; Flux (metallurgy); Very Long Baseline Array; Astronomy; Light curve; Active galactic nucleus; Gamma ray; Galaxy","score_opus":0.016085438863838897,"score_gpt":0.21384509790994713,"score_spread":0.19775965904610823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141145035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99739957,0.00016685242,0.0003651832,0.00005576653,0.000010464879,0.000018594152,0.0008824169,0.00007235697,0.0010288754],"genre_scores_gemma":[0.9932526,0.00016563754,0.00090636505,0.00017071364,0.000043405475,0.000018277236,0.004786883,0.000014809998,0.0006412757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997867,0.000011324068,0.000011353049,0.000047519865,0.00007533625,0.000067816036],"domain_scores_gemma":[0.9996705,0.000020751702,0.00011063368,0.000041073286,0.00007208126,0.00008497599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000256203,0.0002910183,0.00046671275,0.00090246164,0.00035019565,0.00040035203,0.00027425378,0.00040180056,0.00032531391],"category_scores_gemma":[0.0003586595,0.00013821402,0.00024095396,0.00062276924,0.00028512676,0.00023732598,0.0007476905,0.00049685815,0.0002135843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008125639,0.00060044933,0.7502927,0.00015348181,0.0003138896,0.0022508884,0.0009523048,0.0015362642,0.15550798,0.00030297408,0.0042448128,0.08303167],"study_design_scores_gemma":[0.000005728575,0.00007578631,0.9957783,0.0000054570564,0.00002182604,0.00023166781,0.00005517111,0.0003289735,0.0019725813,0.000018196592,0.0015009369,0.0000053458143],"about_ca_topic_score_codex":0.009552102,"about_ca_topic_score_gemma":0.026139988,"teacher_disagreement_score":0.009552102,"about_ca_system_score_codex":0.00067979336,"about_ca_system_score_gemma":0.00033156297,"threshold_uncertainty_score":0.01899296},"labels":[],"label_agreement":null},{"id":"W2141169613","doi":"10.1086/431572","title":"Modeling Complete Distributions with Incomplete Observations: The Velocity Ellipsoid from<i>Hipparcos</i>Data","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Velocity dispersion; Galaxy; Astrophysics; Ellipsoid; Gaussian; Radial velocity; Stars; Halo; Angular velocity; Peculiar velocity; Distribution function; Tensor (intrinsic definition); Geometry; Mathematics; Classical mechanics; Astronomy; Redshift","score_opus":0.05906472315781523,"score_gpt":0.2495633183600848,"score_spread":0.19049859520226958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141169613","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03993146,0.000288994,0.955738,0.00024583103,0.00002971549,0.000058050748,0.0017002055,0.001094405,0.00091342285],"genre_scores_gemma":[0.6008252,0.0007068821,0.3829691,0.00021241559,0.00012044548,0.00028452527,0.01164932,0.00075458473,0.0024774985],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99850285,0.00043848014,0.00008083507,0.000464143,0.00036332358,0.0001504412],"domain_scores_gemma":[0.99518824,0.0020060826,0.0006948822,0.0013104007,0.00064885314,0.00015161526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0053863917,0.0007901159,0.0009720896,0.0026647144,0.000691413,0.0019961835,0.0029343783,0.0010220926,0.0010657415],"category_scores_gemma":[0.018894253,0.0012062415,0.0014008625,0.002564592,0.0011103024,0.0027819804,0.002573076,0.0015144243,0.0007366654],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017237758,0.000053956628,0.037587292,0.00011257771,0.0002184279,0.00018327567,0.00040238,0.8087694,0.0018272355,0.03799248,0.0065421253,0.10613848],"study_design_scores_gemma":[0.000010975098,0.000009497585,0.0059675616,0.000022055501,0.000015979673,0.00006179322,0.000041182277,0.96501297,0.00069241994,0.025358189,0.0027820596,0.000025180394],"about_ca_topic_score_codex":0.028943986,"about_ca_topic_score_gemma":0.01921538,"teacher_disagreement_score":0.028943986,"about_ca_system_score_codex":0.0017110053,"about_ca_system_score_gemma":0.001974007,"threshold_uncertainty_score":0.057551026},"labels":[],"label_agreement":null},{"id":"W2141191349","doi":"10.1088/0004-637x/784/2/93","title":"HOT GALACTIC WINDS CONSTRAINED BY THE X-RAY LUMINOSITIES OF GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Supernova; Luminosity; Galaxy; Adiabatic process; Star formation; Active galactic nucleus; Stellar mass","score_opus":0.006097495621763006,"score_gpt":0.20146930782558706,"score_spread":0.19537181220382405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141191349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948372,0.00012521372,0.0034262554,0.000020875481,0.0000027773701,0.0000071396107,0.000123244,0.000035534373,0.0014217065],"genre_scores_gemma":[0.99905056,0.000084791696,0.00053189293,0.00001636492,0.0000042743645,0.000004355453,0.00017839865,0.0000077504665,0.00012157462],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999665,0.00008313413,0.000026397065,0.00009086145,0.000046601835,0.00008788153],"domain_scores_gemma":[0.99823344,0.0006314943,0.00060917187,0.000306764,0.00006343934,0.00015573167],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006658435,0.00058323704,0.00043306657,0.00061325997,0.0003331781,0.0012972845,0.0005272984,0.0004900904,0.0011301995],"category_scores_gemma":[0.002963801,0.0005284686,0.00047706923,0.00056398544,0.00062577386,0.00074454106,0.00085163297,0.00033889737,0.00025708755],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016838165,0.000037934842,0.9149159,0.00003442284,0.00019214959,0.00024531345,0.00013948324,0.061385456,0.011421776,0.005101248,0.00021010045,0.006147802],"study_design_scores_gemma":[0.00004876128,0.000064725544,0.86154485,0.00004031749,0.00010792925,0.00029414918,0.00019955017,0.1254322,0.0035429297,0.00801058,0.0006740727,0.000039994924],"about_ca_topic_score_codex":0.007716905,"about_ca_topic_score_gemma":0.009106767,"teacher_disagreement_score":0.007716905,"about_ca_system_score_codex":0.0005355546,"about_ca_system_score_gemma":0.00028310737,"threshold_uncertainty_score":0.015343964},"labels":[],"label_agreement":null},{"id":"W2141435988","doi":"10.1086/498057","title":"Space‐ and Ground‐based Pulsation Data of η Bootis Explained with Stellar Models Including Turbulence","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Turbulence; Oscillation (cell signaling); Turbulence kinetic energy; Mode (computer interface); Astrophysics; Space (punctuation); Computational physics; Stars; Kinetic energy; Convection; Energy (signal processing); Mechanics; Classical mechanics","score_opus":0.032279820122292156,"score_gpt":0.2413860289709084,"score_spread":0.20910620884861625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141435988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99733907,0.00003537936,0.0013501048,0.000023186112,0.0000054928546,0.0000040243226,0.00010624659,0.000045896686,0.0010906593],"genre_scores_gemma":[0.9993218,0.00002029641,0.00035563452,0.0000032106386,0.000002557936,0.0000022462468,0.00016287788,0.000009539673,0.00012183631],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999144,0.000018447967,0.000006607375,0.000023839406,0.000018510424,0.000018210034],"domain_scores_gemma":[0.99974555,0.000085252184,0.00006121079,0.000051091127,0.000026560689,0.000030261657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028167316,0.0002847125,0.0002377674,0.00031554367,0.00034621332,0.0004981983,0.00022455162,0.00019713314,0.000569197],"category_scores_gemma":[0.00080274005,0.00015001082,0.00027557008,0.0002698792,0.00021440577,0.00030338007,0.00029666137,0.00020711921,0.00019501256],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044864017,0.00012695775,0.7318597,0.00006189398,0.00013232512,0.00028364046,0.00048354166,0.2068861,0.029133964,0.0068533528,0.0010380342,0.022691848],"study_design_scores_gemma":[0.00009703185,0.00019294227,0.46452376,0.000019588013,0.000081876635,0.00023867251,0.00020133452,0.5195857,0.008560831,0.003521625,0.0029383171,0.00003826408],"about_ca_topic_score_codex":0.008944859,"about_ca_topic_score_gemma":0.0077700117,"teacher_disagreement_score":0.008944859,"about_ca_system_score_codex":0.00054115884,"about_ca_system_score_gemma":0.00025232285,"threshold_uncertainty_score":0.017785609},"labels":[],"label_agreement":null},{"id":"W2141499127","doi":"10.1088/0004-637x/727/2/89","title":"CONVECTIVE-REACTIVE PROTON-<sup>12</sup>C COMBUSTION IN SAKURAI'S OBJECT (V4334 SAGITTARII) AND IMPLICATIONS FOR THE EVOLUTION AND YIELDS FROM THE FIRST GENERATIONS OF STARS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":231,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Nucleosynthesis; Astrophysics; White dwarf; Metallicity; Neutron star; Stellar evolution; Stars; Convection; Convection zone; Supernova; Thermodynamics","score_opus":0.020901684238679708,"score_gpt":0.22959528297862494,"score_spread":0.20869359873994522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141499127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995078,0.00008253314,0.00012868934,0.000012144508,0.0000012670157,0.0000020325824,0.000033792483,0.000011469868,0.00022017506],"genre_scores_gemma":[0.9996076,0.000030141704,0.00018122038,0.00000572219,0.0000012113939,0.0000021366075,0.00009735783,0.0000049548303,0.000069700436],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996877,0.000003705539,0.0000035449596,0.000009800061,0.000004616718,0.000009464871],"domain_scores_gemma":[0.99993634,0.000008461089,0.000025583196,0.0000074181457,0.000005782968,0.000016301354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010978284,0.00036308038,0.00018433231,0.00024256796,0.00033838177,0.0004481276,0.00036330477,0.00035248077,0.00070441805],"category_scores_gemma":[0.00014804032,0.0002293409,0.00033235483,0.0002813755,0.00029816816,0.00020032913,0.00035175486,0.00014888788,0.0001955999],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000598449,0.00011221311,0.5963722,0.00016962945,0.00018085983,0.001794173,0.0006237888,0.04189686,0.34586778,0.0012509034,0.00025663478,0.010876478],"study_design_scores_gemma":[0.00006105151,0.00028309305,0.9033154,0.000016222077,0.00009818831,0.0008857197,0.0005383078,0.069432974,0.023412926,0.00086104113,0.0010565041,0.00003859246],"about_ca_topic_score_codex":0.0060092383,"about_ca_topic_score_gemma":0.0045456304,"teacher_disagreement_score":0.0060092383,"about_ca_system_score_codex":0.00045434493,"about_ca_system_score_gemma":0.00014090941,"threshold_uncertainty_score":0.011948526},"labels":[],"label_agreement":null},{"id":"W2141515548","doi":"10.1088/0004-637x/725/1/1252","title":"STAR FORMATION HISTORIES IN A CLUSTER ENVIRONMENT AT<i>z</i>∼ 0.84","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Star formation; Galaxy; Cluster (spacecraft); Luminosity function; Balmer series; Galaxy cluster; Astronomy; Luminosity; Stellar mass; Stars; Spectral line; Emission spectrum","score_opus":0.004643082849741124,"score_gpt":0.1812452703771902,"score_spread":0.17660218752744908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141515548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987668,0.000018954026,0.000016688915,0.000037978414,9.828499e-7,0.0000024302742,0.0003466465,0.0000058118503,0.0008037524],"genre_scores_gemma":[0.99881977,0.000015953641,0.000041737658,0.000008017857,0.0000013329745,0.0000027472606,0.00048650964,0.000003040923,0.0006209331],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999217,0.000012801496,0.00000321067,0.000020117257,0.000008577871,0.00003355155],"domain_scores_gemma":[0.99931884,0.00008411681,0.00011085421,0.000035085202,0.00010282831,0.0003482105],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001458929,0.00006864455,0.00016230514,0.0005941223,0.00079116505,0.0005901125,0.00020744372,0.00020533889,0.003822925],"category_scores_gemma":[0.00081061985,0.00010289724,0.00008863522,0.0006853016,0.00020898528,0.00027312626,0.000684983,0.00023679438,0.0006357072],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005232603,0.00020424933,0.9782204,0.000018038601,0.000047054193,0.00036930604,0.0013646822,0.0031163394,0.0033564232,0.0010198422,0.0039811386,0.007779237],"study_design_scores_gemma":[0.0000075274443,0.000042828877,0.99602365,0.0000025647453,0.000007874427,0.000060115784,0.00086617307,0.0017064981,0.00020597993,0.00019496879,0.00087529863,0.000006494554],"about_ca_topic_score_codex":0.037202798,"about_ca_topic_score_gemma":0.056341134,"teacher_disagreement_score":0.037202798,"about_ca_system_score_codex":0.00056554243,"about_ca_system_score_gemma":0.00035784545,"threshold_uncertainty_score":0.07397252},"labels":[],"label_agreement":null},{"id":"W2141740237","doi":"10.1088/0004-637x/707/1/283","title":"IONIZED GAS TOWARD MOLECULAR CLUMPS: PHYSICAL PROPERTIES OF MASSIVE STAR-FORMING REGIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; National Radio Astronomy Observatory; National Science Foundation","keywords":"Astrophysics; Physics; Stars; Millimeter; Ionization; Star formation; Star cluster; Power law; Astronomy; Plasma; Cluster (spacecraft); Ion; Nuclear physics","score_opus":0.017434858066690484,"score_gpt":0.2419157597140288,"score_spread":0.2244809016473383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141740237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994492,0.00016839882,0.00020074841,0.000005019885,6.562508e-7,0.000004266648,0.00005347599,0.0000057718,0.000112327245],"genre_scores_gemma":[0.99907315,0.000070049566,0.0004933498,0.000010539876,0.000004958703,0.000003872434,0.000247321,0.0000030192155,0.00009364134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998809,0.000012121094,0.000008049917,0.00003519612,0.000026209618,0.000037416332],"domain_scores_gemma":[0.99945086,0.0001003017,0.0002216708,0.000031148535,0.000061364495,0.00013459676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034395733,0.00018361783,0.00022976333,0.0009973922,0.00033283772,0.00059481914,0.00044671271,0.00017750666,0.0007233232],"category_scores_gemma":[0.0007615964,0.0001841921,0.00011844763,0.0007448696,0.0002631999,0.0002867622,0.000461203,0.00015089453,0.00016886709],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024498437,0.00009015635,0.9354345,0.000041438572,0.000042376858,0.00029758448,0.00041130153,0.00066399097,0.05742467,0.00021669397,0.00009594147,0.005036436],"study_design_scores_gemma":[0.000038165555,0.00022122204,0.98545754,0.000014390257,0.00003415681,0.0006990755,0.00026272648,0.002032093,0.010439267,0.00019563147,0.00059471617,0.000011058654],"about_ca_topic_score_codex":0.0013438066,"about_ca_topic_score_gemma":0.0011353029,"teacher_disagreement_score":0.0013438066,"about_ca_system_score_codex":0.00015959858,"about_ca_system_score_gemma":0.0001040735,"threshold_uncertainty_score":0.002671957},"labels":[],"label_agreement":null},{"id":"W2141774721","doi":"10.1088/0004-637x/702/2/1575","title":"QUARK-NOVAE, COSMIC REIONIZATION, AND EARLY<i>r</i>-PROCESS ELEMENT PRODUCTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Calgary","funders":"","keywords":"Physics; Reionization; Astrophysics; Supernova; Stars; Ejecta; Metallicity; Redshift; Initial mass function; Astronomy; Nucleosynthesis; Universe; Galaxy; Star formation","score_opus":0.0075357749314377016,"score_gpt":0.23166478374518754,"score_spread":0.22412900881374984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2141774721","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94600505,0.0027534147,0.007717677,0.0011495532,0.00005520313,0.000017861397,0.000107870146,0.00007871685,0.0421146],"genre_scores_gemma":[0.99519277,0.00075538177,0.00097265415,0.00008958788,0.000021828395,0.000005694169,0.000070194845,0.0000055065702,0.002886405],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999387,0.000009325479,0.0000032270682,0.000011582108,0.000009024422,0.000028058668],"domain_scores_gemma":[0.99948597,0.00014079585,0.00017104494,0.00003749981,0.000023980727,0.00014061056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018001033,0.00033188908,0.00017840581,0.0003717037,0.000499526,0.0010608884,0.00042537155,0.000624085,0.0031388705],"category_scores_gemma":[0.0005847519,0.00011203949,0.00034279324,0.00033012536,0.00046240253,0.0007874494,0.00080511405,0.00040498306,0.0002781365],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003661218,0.0002361127,0.35665178,0.00023440385,0.00009286435,0.00664034,0.0007715369,0.021096544,0.022180213,0.5488778,0.0022813648,0.040570825],"study_design_scores_gemma":[0.00013650057,0.00047157978,0.43337107,0.00016140644,0.000121990255,0.00800548,0.0012654851,0.13242647,0.014224721,0.36626428,0.043461755,0.000089221045],"about_ca_topic_score_codex":0.0029187708,"about_ca_topic_score_gemma":0.0024469097,"teacher_disagreement_score":0.0031388705,"about_ca_system_score_codex":0.0005017928,"about_ca_system_score_gemma":0.0002310068,"threshold_uncertainty_score":0.01050055},"labels":[],"label_agreement":null},{"id":"W2142191033","doi":"10.1086/499916","title":"Identification of the Red Supergiant Progenitor of Supernova 2005cs: Do the Progenitors of Type II‐P Supernovae Have Low Mass?","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":161,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Red supergiant; Supernova; Physics; Astrophysics; Supergiant; Advanced Camera for Surveys; Stars; Photometry (optics); Astronomy; Galaxy; Brightness; Hubble space telescope","score_opus":0.007185447778737043,"score_gpt":0.21760878956289734,"score_spread":0.2104233417841603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142191033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965397,0.00094089843,0.0007185263,0.00005528991,0.000004939402,0.000008275193,0.00008053854,0.000017264247,0.0016345296],"genre_scores_gemma":[0.9976119,0.00063386513,0.0006925151,0.00004329105,0.000015049852,0.0000037250784,0.00041318516,0.0000047556864,0.0005817974],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992263,0.000007101139,0.000008457352,0.000026056838,0.000018950046,0.00001679435],"domain_scores_gemma":[0.999678,0.00003065323,0.0001405732,0.0000249761,0.00006528389,0.000060408314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039566966,0.00017673099,0.00020920938,0.0007486448,0.00031033673,0.0009011793,0.00029578476,0.0003156836,0.0012908458],"category_scores_gemma":[0.00060552836,0.00009040255,0.00010033459,0.00048522913,0.0003140413,0.00057560357,0.00036256295,0.00018051497,0.0004847583],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008765785,0.00001965597,0.96526515,0.00004567601,0.000013821422,0.00076588476,0.00023605855,0.00005320587,0.015074458,0.0002722677,0.00011967679,0.01804653],"study_design_scores_gemma":[0.0000031734064,0.000078807614,0.99085695,0.000029898249,0.000012507906,0.0017471374,0.000637472,0.00038381197,0.003951674,0.0001948133,0.0020997082,0.0000039723877],"about_ca_topic_score_codex":0.003287886,"about_ca_topic_score_gemma":0.0062751514,"teacher_disagreement_score":0.003287886,"about_ca_system_score_codex":0.00022894,"about_ca_system_score_gemma":0.00024356286,"threshold_uncertainty_score":0.006537497},"labels":[],"label_agreement":null},{"id":"W2142235810","doi":"10.1088/0004-637x/799/2/208","title":"TOWARD CHARACTERIZATION OF THE TYPE IIP SUPERNOVA PROGENITOR POPULATION: A STATISTICAL SAMPLE OF LIGHT CURVES FROM Pan-STARRS1","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":211,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Engineering and Physical Sciences Research Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; Queen's University; Johns Hopkins University; Queen's University Belfast; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Light curve; Supernova; Astrophysics; Red supergiant; Physics; Population; Luminosity; Cosmic distance ladder; Astronomy; Supergiant; Stars; Redshift; Galaxy","score_opus":0.025873008013884577,"score_gpt":0.24856880578149926,"score_spread":0.22269579776761467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142235810","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932231,0.00015141664,0.0049437,0.000016835384,0.0000019764257,0.000025163909,0.00090421294,0.00013332671,0.00060017797],"genre_scores_gemma":[0.98846346,0.000115062474,0.0056263953,0.000014466565,0.00001118587,0.00003028064,0.0054947655,0.000058611888,0.00018567513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994512,0.00008836365,0.000053830125,0.00021291325,0.0001508037,0.00004278104],"domain_scores_gemma":[0.9975637,0.00039912225,0.00067696854,0.00068801036,0.0004167054,0.00025546615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017290892,0.00038457938,0.0004993201,0.002614675,0.0004400631,0.0009849374,0.0004930149,0.00025190655,0.0007924998],"category_scores_gemma":[0.0038913463,0.00019614094,0.000520059,0.0011361847,0.00032160606,0.0005810512,0.0010652879,0.0004240066,0.000580587],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000068594156,0.000028746512,0.976077,0.000017853132,0.000060777485,0.000034914792,0.00010920872,0.00084646314,0.008977733,0.000118555115,0.00013093541,0.013529158],"study_design_scores_gemma":[0.0000027809506,0.000053688054,0.9916175,0.0000055823307,0.000016818945,0.00020673644,0.00008305461,0.005621043,0.0016185709,0.00012240624,0.0006452568,0.0000064917863],"about_ca_topic_score_codex":0.0025360014,"about_ca_topic_score_gemma":0.002243519,"teacher_disagreement_score":0.002614675,"about_ca_system_score_codex":0.00024619623,"about_ca_system_score_gemma":0.00024194062,"threshold_uncertainty_score":0.009144366},"labels":[],"label_agreement":null},{"id":"W2142549464","doi":"10.1088/0004-637x/757/1/10","title":"CONSTRAINTS ON THE COMPACT OBJECT MASS IN THE ECLIPSING HIGH-MASS X-RAY BINARY XMMU J013236.7+303228 IN M 33","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Neutron star; Roche lobe; RADIUS; Millisecond pulsar; Binary number; Orbital period; Compact star; Binary star; X-ray binary; Pulsar","score_opus":0.023917024229646124,"score_gpt":0.2524167931804868,"score_spread":0.2284997689508407,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142549464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990582,0.00016021762,0.00013100496,0.000019452957,0.0000019130473,0.0000028622276,0.000075630865,0.000008873489,0.000541849],"genre_scores_gemma":[0.999376,0.00006633651,0.0002540277,0.000014808525,0.0000050027197,0.0000039082315,0.00017908451,0.0000031351215,0.00009785051],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984217,0.000020295865,0.000013952603,0.000035480636,0.00004758509,0.00004051579],"domain_scores_gemma":[0.9991708,0.000096961216,0.0004280162,0.000052972915,0.00004593159,0.000205365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028308982,0.00047173837,0.0005002827,0.0007331514,0.0006237719,0.0008667673,0.00044154812,0.000607062,0.0014841394],"category_scores_gemma":[0.0012220173,0.0002896887,0.00022620586,0.0006354643,0.00043976723,0.00036457164,0.0010161191,0.00035891315,0.0006400534],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000618129,0.00006902369,0.9018457,0.00009044984,0.000052968095,0.001628522,0.0005899207,0.000863801,0.08446671,0.000779277,0.00031590095,0.008679621],"study_design_scores_gemma":[0.000013507661,0.00009455645,0.99587446,0.00002111323,0.000018192204,0.00061958405,0.00023541867,0.00084984186,0.0014431207,0.000219059,0.00060108356,0.0000100866455],"about_ca_topic_score_codex":0.003144266,"about_ca_topic_score_gemma":0.008182479,"teacher_disagreement_score":0.003144266,"about_ca_system_score_codex":0.00043399498,"about_ca_system_score_gemma":0.00020431493,"threshold_uncertainty_score":0.006251931},"labels":[],"label_agreement":null},{"id":"W2142714210","doi":"10.1086/378156","title":"Coordinated Multiwavelength Observations of BL Lacertae in 2000","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Blazar; Astrophysics; Telescope; Observatory; Light curve; Flux (metallurgy); BL Lac object; Active galactic nucleus; Synchrotron; Astronomy; Gamma ray; Galaxy; Optics","score_opus":0.015287561165611785,"score_gpt":0.22720444278470098,"score_spread":0.2119168816190892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142714210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99022526,0.000955727,0.00092228956,0.00014845545,0.00003157599,0.000051702533,0.0025174168,0.00033512176,0.0048125265],"genre_scores_gemma":[0.9887503,0.00032514925,0.0019176736,0.00014489787,0.000057758483,0.000032895485,0.0069787004,0.000050489383,0.0017422353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996698,0.000015074024,0.000011836251,0.000111659225,0.00011303255,0.00007870336],"domain_scores_gemma":[0.99957055,0.000016823298,0.00012372002,0.000050937404,0.000085052125,0.000152904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047614923,0.00036785527,0.00042855556,0.0017908248,0.0004094849,0.0011185574,0.00034914256,0.0004820121,0.00064120215],"category_scores_gemma":[0.00046417722,0.00023069054,0.0003080378,0.0010508638,0.00013882013,0.00035482872,0.00087987864,0.00054165244,0.00033527502],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024840233,0.0004632204,0.48643407,0.00020759633,0.0005861219,0.0012038008,0.0019062404,0.003944513,0.40319282,0.0006811386,0.006857356,0.09203906],"study_design_scores_gemma":[0.000031615386,0.00007502316,0.9925383,0.000007983367,0.00004263629,0.00009524359,0.00007616951,0.00067202083,0.0030911176,0.000071946095,0.0032894188,0.000008520006],"about_ca_topic_score_codex":0.014717228,"about_ca_topic_score_gemma":0.031419817,"teacher_disagreement_score":0.014717228,"about_ca_system_score_codex":0.001518279,"about_ca_system_score_gemma":0.0003179286,"threshold_uncertainty_score":0.029263139},"labels":[],"label_agreement":null},{"id":"W2142756928","doi":"10.1088/0004-637x/733/1/28","title":"IMPROVED ORBITAL PARAMETERS AND TRANSIT MONITORING FOR HD 156846b","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Ephemeris; Transit (satellite); Jovian; Photometry (optics); Radial velocity; Spectrometer; Planet; Exoplanet; Orbital decay","score_opus":0.024641397360365053,"score_gpt":0.2268038805120318,"score_spread":0.20216248315166674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142756928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99018645,0.00007993934,0.0016946577,0.00007385211,0.000021757356,0.000022476608,0.005050752,0.00014366198,0.0027265646],"genre_scores_gemma":[0.98583674,0.000027842141,0.0057452274,0.000030350486,0.000018219385,0.00002095415,0.00720161,0.000048545655,0.0010704681],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997861,0.00002898465,0.000016301952,0.00008304158,0.000054003423,0.000031607648],"domain_scores_gemma":[0.99955124,0.000041998574,0.000110985464,0.00012893215,0.000081329374,0.00008544519],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041881364,0.0002315155,0.000342431,0.0009262961,0.00045120541,0.00028598818,0.00024478274,0.0004580987,0.0018742281],"category_scores_gemma":[0.00086852786,0.000155741,0.00019899027,0.0007422365,0.00010282044,0.0002393338,0.00033509766,0.00043343127,0.0010708353],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005132513,0.00024907227,0.73719996,0.000114865725,0.00006657505,0.00062222005,0.00046643146,0.0040322747,0.21424332,0.0005616935,0.004249842,0.037680496],"study_design_scores_gemma":[0.000016602491,0.00008067311,0.9866384,0.0000063457273,0.000020041522,0.00027846493,0.000039445564,0.0020304208,0.0059237094,0.00009206482,0.004861262,0.000012643743],"about_ca_topic_score_codex":0.0037286705,"about_ca_topic_score_gemma":0.010326417,"teacher_disagreement_score":0.0037286705,"about_ca_system_score_codex":0.000364121,"about_ca_system_score_gemma":0.00016642967,"threshold_uncertainty_score":0.0074139237},"labels":[],"label_agreement":null},{"id":"W2142779957","doi":"10.1088/0004-637x/785/2/149","title":"THE REST-FRAME SUBMILLIMETER SPECTRUM OF HIGH-REDSHIFT, DUSTY, STAR-FORMING GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":144,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Dalhousie University","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Commonwealth Scientific and Industrial Research Organisation; Gordon and Betty Moore Foundation; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Star formation; Emission spectrum; Astronomy; Interstellar medium; Line (geometry); Spectral line; Rest frame","score_opus":0.007733037637734652,"score_gpt":0.21865257757362028,"score_spread":0.21091953993588564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142779957","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951402,0.000101308775,0.00041404384,0.000028766852,0.0000041092394,0.000005165129,0.0020225884,0.0001223826,0.0021613713],"genre_scores_gemma":[0.9961313,0.000075774,0.000508766,0.000032531207,0.000018630093,0.000005350286,0.00265895,0.000014735509,0.0005539043],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999572,0.0000036478737,0.0000019045522,0.000011268103,0.000009059581,0.000016858769],"domain_scores_gemma":[0.99980706,0.000025097714,0.000042931744,0.000016534497,0.00002438821,0.000084025654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011440841,0.00019688293,0.00014692893,0.00074217364,0.00017484683,0.00029361178,0.00017368534,0.000141213,0.002817445],"category_scores_gemma":[0.00017964767,0.00007629198,0.00014940697,0.000527309,0.00008490524,0.00016077592,0.00018840883,0.00013276667,0.0004369669],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014919859,0.000071655595,0.9050994,0.000049092298,0.00011885421,0.00027624628,0.00029625988,0.0010896844,0.064164564,0.00048019856,0.0029497447,0.025255008],"study_design_scores_gemma":[0.000001964942,0.00001747305,0.998231,0.0000012477575,0.0000089534215,0.00010222609,0.000024102002,0.00033252282,0.0006117264,0.00003322719,0.00063397124,0.0000015331998],"about_ca_topic_score_codex":0.0023469497,"about_ca_topic_score_gemma":0.003058913,"teacher_disagreement_score":0.002817445,"about_ca_system_score_codex":0.00016756197,"about_ca_system_score_gemma":0.000041391806,"threshold_uncertainty_score":0.009425342},"labels":[],"label_agreement":null},{"id":"W2142811991","doi":"10.1088/0004-637x/741/2/76","title":"PTF 10bzf (SN 2010ah): A BROAD-LINE Ic SUPERNOVA DISCOVERED BY THE PALOMAR TRANSIENT FACTORY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gamma-ray burst; Supernova; Luminosity; Telescope; Kinetic energy; Transient (computer programming)","score_opus":0.0193348674467768,"score_gpt":0.2232189519975066,"score_spread":0.20388408455072982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142811991","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99556655,0.00017431323,0.00042092043,0.00012335683,0.000024681367,0.000029308336,0.0010701631,0.000066014734,0.0025246884],"genre_scores_gemma":[0.9949463,0.00018411595,0.000914283,0.0001315983,0.000032769625,0.00001726734,0.002222656,0.000014209093,0.0015368536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991083,0.0000035565683,0.0000039433457,0.000029126544,0.000021748634,0.000030820967],"domain_scores_gemma":[0.9996706,0.000016334257,0.00010717322,0.000033888973,0.000033158598,0.0001388947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017631003,0.00040017976,0.0002813098,0.0008879361,0.00065972557,0.00054658874,0.00034372672,0.00040762615,0.0020095233],"category_scores_gemma":[0.00020296469,0.00020500572,0.00023679528,0.00045323433,0.00034576788,0.00037683072,0.0007483203,0.00048091408,0.0005735338],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071429426,0.00020009707,0.9231609,0.000084001374,0.00011925028,0.010081006,0.0003720171,0.00024498877,0.035254877,0.00037164582,0.003906255,0.025490861],"study_design_scores_gemma":[0.000038206555,0.0003209128,0.9790754,0.0000143418265,0.000027238855,0.010275721,0.00024407147,0.00044575628,0.0027377508,0.00012455352,0.0066812513,0.00001490711],"about_ca_topic_score_codex":0.013433297,"about_ca_topic_score_gemma":0.020395178,"teacher_disagreement_score":0.013433297,"about_ca_system_score_codex":0.00050480006,"about_ca_system_score_gemma":0.00025717384,"threshold_uncertainty_score":0.026710212},"labels":[],"label_agreement":null},{"id":"W2142830639","doi":"10.1086/422635","title":"Determining Foreground Contamination in Cosmic Microwave Background Observations: Diffuse Galactic Emission in the MAXIMA‐I Field","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Astrophysics; Maxima; Astronomy; Amplitude; Synchrotron radiation; Microwave; Cosmic ray; Synchrotron; Spectral density; Optics","score_opus":0.02271035128475198,"score_gpt":0.27002232360640693,"score_spread":0.24731197232165494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142830639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9576182,0.00039550013,0.038934857,0.000066423156,0.000009272363,0.000026170706,0.00044489437,0.00029451624,0.0022101572],"genre_scores_gemma":[0.9825013,0.00024891758,0.01615503,0.000027388653,0.00002867346,0.000022523749,0.00077291933,0.000066465785,0.00017674532],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994004,0.0001774109,0.000043037482,0.00014446558,0.00015058018,0.000084169085],"domain_scores_gemma":[0.99732673,0.0013393243,0.00053373707,0.00050357514,0.00019433741,0.00010230359],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00109932,0.0005011363,0.00047237036,0.0018937864,0.00036829477,0.0008876798,0.00043515864,0.00047593596,0.0005289143],"category_scores_gemma":[0.0070538255,0.00040310842,0.0004611212,0.0020055682,0.00048401006,0.00058003975,0.0009976646,0.00032537908,0.00023175734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044445766,0.000089818845,0.85172546,0.0001888241,0.00023787859,0.00054907333,0.00044647962,0.014385071,0.045209862,0.002827974,0.00049826055,0.08339696],"study_design_scores_gemma":[0.000043884756,0.00006680455,0.92867374,0.000038844308,0.00015946789,0.00064420287,0.00015091753,0.040460143,0.024697928,0.0032006272,0.001837092,0.000026262478],"about_ca_topic_score_codex":0.0030138274,"about_ca_topic_score_gemma":0.0037321954,"teacher_disagreement_score":0.0030138274,"about_ca_system_score_codex":0.000400146,"about_ca_system_score_gemma":0.00030373925,"threshold_uncertainty_score":0.005992532},"labels":[],"label_agreement":null},{"id":"W2142889681","doi":"10.1088/0004-637x/706/2/1353","title":"DETECTING CHANGING POLARIZATION STRUCTURES IN SAGITTARIUS A* WITH HIGH FREQUENCY VLBI","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Very-long-baseline interferometry; Physics; Polarization (electrochemistry); Linear polarization; Supermassive black hole; Astrophysics; Polarimetry; Polarization in astronomy; Schwarzschild radius; Millimeter; Faraday effect; Galactic Center; Astronomy; Accretion (finance); Optics; Stars; Galaxy; Scattering; Magnetic field","score_opus":0.0069842607192402316,"score_gpt":0.21041501445020547,"score_spread":0.20343075373096522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142889681","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99454725,0.000055057153,0.0032946703,0.00010819845,0.000011911362,0.00001174962,0.00035721806,0.00018807102,0.0014260332],"genre_scores_gemma":[0.99754024,0.00003412133,0.0015668527,0.000039621544,0.0000057011703,0.0000109354105,0.0006082327,0.00003974852,0.00015463174],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998271,0.000045263558,0.000008476358,0.000041700852,0.000030842937,0.000046670768],"domain_scores_gemma":[0.9997296,0.000081085025,0.000042248368,0.000046786,0.00004674791,0.000053495838],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039512027,0.0003824317,0.00034669094,0.00038180844,0.0002824186,0.00095550384,0.0008581787,0.00064655166,0.00079459],"category_scores_gemma":[0.0009723433,0.00031452373,0.0005969338,0.00046006395,0.0004049049,0.00055981305,0.00057639554,0.0004331056,0.00021969683],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035897776,0.00030497354,0.1554193,0.000049453327,0.0003277335,0.00022809986,0.00018229656,0.8103632,0.020179758,0.0017498925,0.0013447719,0.009491612],"study_design_scores_gemma":[0.00006334958,0.00009945514,0.053752635,0.000008040841,0.000042957407,0.000052980755,0.000086914246,0.94163686,0.00270805,0.000708253,0.00080917816,0.00003134208],"about_ca_topic_score_codex":0.016989434,"about_ca_topic_score_gemma":0.0089111775,"teacher_disagreement_score":0.016989434,"about_ca_system_score_codex":0.00073184195,"about_ca_system_score_gemma":0.00041368033,"threshold_uncertainty_score":0.03378111},"labels":[],"label_agreement":null},{"id":"W2142983399","doi":"10.1088/0004-637x/768/1/85","title":"THE PULSAR SEARCH COLLABORATORY: DISCOVERY AND TIMING OF FIVE NEW PULSARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Millisecond pulsar; Observatory; Telescope; White dwarf; Astrometry; Radio telescope; Pulsar planet","score_opus":0.012565497372517892,"score_gpt":0.30111023791868374,"score_spread":0.28854474054616586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2142983399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88415885,0.0015963019,0.06037755,0.0051801386,0.000699204,0.00042384161,0.010390427,0.0060487874,0.031124895],"genre_scores_gemma":[0.8592507,0.0008429917,0.11218919,0.00057372404,0.0005132045,0.00022861248,0.014557959,0.0007780288,0.011065499],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.999199,0.00008517064,0.00004562492,0.00019339868,0.00038068788,0.000096152326],"domain_scores_gemma":[0.9971915,0.00061082427,0.00042908525,0.0005264779,0.0004725397,0.000769575],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021631564,0.00042531983,0.00037022843,0.0027410446,0.0011709727,0.0013955196,0.0009646298,0.0009411676,0.0038306655],"category_scores_gemma":[0.004522052,0.00026762058,0.00043329844,0.0023375289,0.00055063545,0.0010801645,0.0019315172,0.0009773024,0.0008729521],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015370273,0.00070858945,0.32409972,0.00037790535,0.00019130229,0.0026442925,0.0064314036,0.0077156387,0.041804034,0.010320714,0.11306112,0.49110824],"study_design_scores_gemma":[0.00070601044,0.0017817855,0.4105777,0.00022399177,0.00028400644,0.006791657,0.0040688426,0.06594627,0.047453895,0.012439743,0.44931084,0.00041519137],"about_ca_topic_score_codex":0.003570231,"about_ca_topic_score_gemma":0.006202673,"teacher_disagreement_score":0.0038306655,"about_ca_system_score_codex":0.0005971253,"about_ca_system_score_gemma":0.0012101572,"threshold_uncertainty_score":0.012814879},"labels":[],"label_agreement":null},{"id":"W2143021331","doi":"10.1088/0004-637x/756/1/48","title":"A NEW TYPE OF AMBIGUITY IN THE PLANET AND BINARY INTERPRETATIONS OF CENTRAL PERTURBATIONS OF HIGH-MAGNIFICATION GRAVITATIONAL MICROLENSING EVENTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Japan Society for the Promotion of Science; National Research Foundation of Korea; Fonds De La Recherche Scientifique - FNRS; Fonds National de la Recherche Luxembourg; Qatar National Research Fund; Qatar Foundation; Korea Research Council of Fundamental Science and Technology; Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; California Institute of Technology; European Commission; Fédération Wallonie-Bruxelles; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Science Foundation","keywords":"Gravitational microlensing; Perturbation (astronomy); Binary number; Planet; Binary Independence Model; Degeneracy (biology); Light curve; Binary star","score_opus":0.015184200475006494,"score_gpt":0.24865633054863354,"score_spread":0.23347213007362705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143021331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9495869,0.00064985495,0.032586247,0.0004682424,0.00005778091,0.00003751827,0.00025142127,0.00041090685,0.01595113],"genre_scores_gemma":[0.9955591,0.00004291424,0.0039160666,0.000025784899,0.000024981284,0.0000026478726,0.00009555415,0.00002372715,0.00030922866],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995414,0.00006536511,0.000040218998,0.00012171232,0.00015403438,0.000077176854],"domain_scores_gemma":[0.99856734,0.0004167877,0.00045167422,0.00032615382,0.00011996893,0.00011803039],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060231244,0.00029336027,0.00034075,0.0011932832,0.0007813925,0.0014094583,0.0004251149,0.0008835028,0.001758669],"category_scores_gemma":[0.002420299,0.00023143008,0.0003747497,0.00067363237,0.0014718896,0.0014279833,0.0013009706,0.00076390494,0.00016607267],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002196716,0.00019559311,0.51021725,0.00045920943,0.00016836372,0.024977457,0.009206253,0.017388102,0.17394309,0.15239775,0.004137734,0.10471255],"study_design_scores_gemma":[0.00013529554,0.00022859208,0.65840024,0.00015446935,0.000121103854,0.028453331,0.0019316018,0.16384883,0.041685276,0.08450124,0.020350441,0.00018961824],"about_ca_topic_score_codex":0.0010898354,"about_ca_topic_score_gemma":0.0007439854,"teacher_disagreement_score":0.001758669,"about_ca_system_score_codex":0.0005150327,"about_ca_system_score_gemma":0.00024826915,"threshold_uncertainty_score":0.005883336},"labels":[],"label_agreement":null},{"id":"W2143403649","doi":"10.1088/0004-637x/780/1/97","title":"RESOLVED IMAGING OF THE HR 8799 DEBRIS DISK WITH HERSCHEL *","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Planetesimal; Debris disk; Astrophysics; Physics; Planetary system; Planet; Halo; Thick disk; Astronomy; Black-body radiation; Debris; Galaxy","score_opus":0.006564797889118707,"score_gpt":0.200807554833471,"score_spread":0.1942427569443523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143403649","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9597121,0.000867283,0.0013831303,0.00055331143,0.000032564545,0.000052488966,0.0043932446,0.0004372948,0.032568607],"genre_scores_gemma":[0.988525,0.00028840025,0.0045484933,0.00034193875,0.000038509625,0.000021904489,0.002552239,0.000080451464,0.0036030253],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.000010972227,0.0000050126982,0.000031172956,0.000046884332,0.000028192355],"domain_scores_gemma":[0.9998135,0.000027427901,0.00002863923,0.00004659098,0.000050304272,0.000033599757],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003482613,0.00012052752,0.00016835728,0.00081144215,0.00036175316,0.00048338625,0.0003188617,0.00037859296,0.00218162],"category_scores_gemma":[0.00032145798,0.00014889214,0.0001829293,0.0004650725,0.00018220305,0.00039963002,0.00046577593,0.0003618028,0.0004969635],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011691406,0.0005243991,0.178962,0.00028876806,0.00032094968,0.0019942143,0.0010879115,0.0061207074,0.7226636,0.003812973,0.021421095,0.061634265],"study_design_scores_gemma":[0.0001194186,0.00017486181,0.93523186,0.00006880226,0.00007512805,0.0007139074,0.00044231577,0.008267015,0.028382415,0.0009991924,0.025482073,0.000043016447],"about_ca_topic_score_codex":0.0037373102,"about_ca_topic_score_gemma":0.011283616,"teacher_disagreement_score":0.0037373102,"about_ca_system_score_codex":0.0006950658,"about_ca_system_score_gemma":0.00030883672,"threshold_uncertainty_score":0.00743109},"labels":[],"label_agreement":null},{"id":"W2143443900","doi":"10.1088/0004-637x/786/1/70","title":"FOMALHAUT b AS A CLOUD OF DUST: TESTING ASPECTS OF PLANET FORMATION THEORY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Planetary system; Range (aeronautics); Cascade; Cloud computing; Debris","score_opus":0.0087647549900189,"score_gpt":0.20269992395698808,"score_spread":0.19393516896696916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143443900","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945932,0.00008494404,0.0028585456,0.00020146628,0.000005719106,0.000018773466,0.000045664943,0.000025578947,0.002166052],"genre_scores_gemma":[0.99880266,0.000039724386,0.0009509109,0.000015448104,0.0000068644426,0.000006023141,0.00002509628,0.000005653428,0.00014758964],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99981374,0.000054782024,0.000007712396,0.00003695865,0.000030933104,0.000055767752],"domain_scores_gemma":[0.99726474,0.0016805225,0.00036916003,0.00017792445,0.00011379618,0.00039395547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068451697,0.0004936596,0.0004391611,0.0007471218,0.000958896,0.0011601571,0.0012449833,0.0008138166,0.0012227107],"category_scores_gemma":[0.003817249,0.00020503701,0.00071237265,0.0003970363,0.0011350022,0.0014096515,0.0009962883,0.00041426436,0.000099281395],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072990597,0.00025926658,0.29552335,0.00011513275,0.00025728488,0.0020326392,0.000813105,0.5990249,0.0048238225,0.08323997,0.0011472546,0.012033367],"study_design_scores_gemma":[0.00010289263,0.00009873011,0.019226119,0.000007441563,0.000022936782,0.00021285412,0.0002369935,0.9630188,0.0005491986,0.016122606,0.00038306764,0.000018406738],"about_ca_topic_score_codex":0.033964086,"about_ca_topic_score_gemma":0.008755761,"teacher_disagreement_score":0.033964086,"about_ca_system_score_codex":0.0019316989,"about_ca_system_score_gemma":0.0005976588,"threshold_uncertainty_score":0.06753284},"labels":[],"label_agreement":null},{"id":"W2143468430","doi":"10.1086/587951","title":"The ACS Virgo Cluster Survey. XV. The Formation Efficiencies of Globular Clusters in Early‐Type Galaxies: The Effects of Mass and Environment","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":351,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Virgo Cluster; Dwarf galaxy; Galaxy; Astronomy; Star formation; Elliptical galaxy; Stars; Stellar mass; Star cluster","score_opus":0.006105139538613252,"score_gpt":0.18606066187371173,"score_spread":0.17995552233509848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143468430","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.042338468,0.0017220307,0.000762305,0.0005164244,0.00016254651,0.00016095595,0.9426925,0.0012395033,0.010405239],"genre_scores_gemma":[0.06946086,0.0011387132,0.0021878625,0.00026838278,0.00013248382,0.00017014294,0.9209169,0.0002215608,0.005503106],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99945027,0.00007269649,0.000048809747,0.00009595882,0.0002297649,0.0001024872],"domain_scores_gemma":[0.9977076,0.00015892646,0.0005696219,0.0002785923,0.00086559984,0.00041960846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011516415,0.0011909425,0.0009622038,0.009979414,0.0005718638,0.001341331,0.0015123448,0.0005668857,0.009874152],"category_scores_gemma":[0.0027338825,0.0004962459,0.0005364065,0.012035763,0.00025588294,0.0010736223,0.0017772517,0.0008604127,0.007991234],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034628154,0.00021109678,0.23931271,0.0007186595,0.00051464565,0.00014431783,0.0002905446,0.00076474604,0.0014598247,0.0021257508,0.7087817,0.045329608],"study_design_scores_gemma":[0.00020428703,0.000058611826,0.8103095,0.00010373853,0.00014127829,0.00017591138,0.00026166314,0.00071578566,0.0006700943,0.0011163926,0.1862034,0.00003933661],"about_ca_topic_score_codex":0.072340764,"about_ca_topic_score_gemma":0.063577354,"teacher_disagreement_score":0.072340764,"about_ca_system_score_codex":0.001323659,"about_ca_system_score_gemma":0.0010439228,"threshold_uncertainty_score":0.14383936},"labels":[],"label_agreement":null},{"id":"W2143594155","doi":"10.1088/0004-637x/708/1/93","title":"DISCOVERY OF A MULTIPOLAR STRUCTURE WITH AN EQUATORIAL DISK IN NGC 6072","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Hubble sequence; Astronomy; Galaxy; Galaxy formation and evolution","score_opus":0.0063062983798956715,"score_gpt":0.21828753303470752,"score_spread":0.21198123465481186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143594155","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987852,0.0001249371,0.000118412,0.000026004795,0.0000055816286,0.00000246966,0.000057057463,0.000014018544,0.0008663129],"genre_scores_gemma":[0.9992725,0.00003717408,0.00031432213,0.000018128778,0.00000764319,0.0000020411865,0.00013732043,0.0000031334996,0.00020773007],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999928,0.000004029559,0.000004847891,0.000023717728,0.000016726288,0.000022687107],"domain_scores_gemma":[0.99975973,0.000013758229,0.000097102704,0.000024095996,0.000025286558,0.00007999709],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012853218,0.00021444216,0.00021307357,0.000891089,0.0006860057,0.00069158763,0.0003081265,0.00056482037,0.001217371],"category_scores_gemma":[0.00035321948,0.00022149683,0.00012011013,0.00050243223,0.00044734398,0.00038239325,0.0004516293,0.00025551725,0.00032283668],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005274796,0.00016745635,0.645778,0.00006743855,0.00006816079,0.00801099,0.0015520013,0.0008377426,0.31885085,0.0011501958,0.0013772134,0.021612499],"study_design_scores_gemma":[0.000030204377,0.00014662555,0.98601544,0.000012923052,0.00003192717,0.0036391995,0.00045042997,0.00067084277,0.0044728993,0.00031911483,0.004192879,0.000017647824],"about_ca_topic_score_codex":0.0061326344,"about_ca_topic_score_gemma":0.009534565,"teacher_disagreement_score":0.0061326344,"about_ca_system_score_codex":0.0005499675,"about_ca_system_score_gemma":0.00015911204,"threshold_uncertainty_score":0.012193859},"labels":[],"label_agreement":null},{"id":"W2143782024","doi":"10.1086/520843","title":"Self‐Consistent Massive Disks in Triaxial Dark Matter Halos","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Halo; Cuspy halo problem; Physics; Astrophysics; Dark matter halo; Dark matter; Galaxy rotation curve; Surface brightness; Galactic halo; Thick disk; Galaxy; Astronomy","score_opus":0.007660370886389093,"score_gpt":0.22083592287615358,"score_spread":0.21317555198976448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143782024","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96030414,0.00035083975,0.03149844,0.00044978355,0.000039662285,0.000029603134,0.00016652423,0.00025405138,0.0069069453],"genre_scores_gemma":[0.9945563,0.000086145315,0.0036930875,0.000055063007,0.000026413149,0.000024736188,0.0001250192,0.00006742981,0.0013658679],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986565,0.000048691785,0.000008346746,0.000021611031,0.000019252398,0.00003639036],"domain_scores_gemma":[0.99925536,0.00015771066,0.00018778072,0.000091070026,0.00009331882,0.00021478122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005469413,0.00042991873,0.00055322907,0.0007569437,0.0006618044,0.0015919905,0.0015516026,0.0008365063,0.001500027],"category_scores_gemma":[0.0021412494,0.0007490648,0.0005001992,0.00035266715,0.001225181,0.0012342659,0.0017975201,0.00037986552,0.0002854959],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003133854,0.000085529726,0.01993901,0.000068734764,0.00011864394,0.0012462003,0.00022143759,0.89003724,0.0076795137,0.07536253,0.0012968063,0.003631012],"study_design_scores_gemma":[0.00006836753,0.000021009026,0.0034066516,0.0000074209606,0.00001196516,0.000073999036,0.00007090675,0.97771955,0.0004595198,0.017808404,0.00033506184,0.000017212948],"about_ca_topic_score_codex":0.004982303,"about_ca_topic_score_gemma":0.0037639742,"teacher_disagreement_score":0.004982303,"about_ca_system_score_codex":0.0008771744,"about_ca_system_score_gemma":0.00041306557,"threshold_uncertainty_score":0.00990659},"labels":[],"label_agreement":null},{"id":"W2143862555","doi":"10.1086/321328","title":"A Radio Supernova Remnant Associated with the Young Pulsar J1119−6127","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Pulsar wind nebula; Supernova remnant; Astronomy; Astrophysics; Supernova; Nebula; Pulsar planet; Binary pulsar; Millisecond pulsar; Stars","score_opus":0.012161623244925378,"score_gpt":0.2805649300197103,"score_spread":0.2684033067747849,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143862555","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99880326,0.0001178858,0.000112173744,0.000016915219,0.0000055965797,0.0000070718934,0.0000651708,0.0000060461425,0.0008659634],"genre_scores_gemma":[0.99814534,0.00018203049,0.00031593404,0.000034062254,0.000019706782,0.0000066753423,0.0005829624,0.000004803037,0.00070831284],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998783,0.000008530363,0.0000083844125,0.000026288179,0.000039588413,0.000039009123],"domain_scores_gemma":[0.9995851,0.000034470882,0.00017153336,0.00005119431,0.00004380494,0.00011377675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019471119,0.00022993665,0.00028282788,0.0006977747,0.00062010455,0.00055385137,0.00033251423,0.00023661945,0.0010436967],"category_scores_gemma":[0.00045893213,0.00023576798,0.00015403079,0.0004378064,0.00051370496,0.00023336781,0.00087784335,0.00032597955,0.00047822658],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032189142,0.00023849052,0.88970757,0.0001054476,0.00010181914,0.018273747,0.00081905746,0.00019658635,0.0729655,0.00046010272,0.0009744309,0.01583544],"study_design_scores_gemma":[0.00002052466,0.00026361312,0.97724867,0.0000098758,0.00004516181,0.014178158,0.00026663404,0.00022314276,0.0039496743,0.000089894,0.0036926619,0.000012013158],"about_ca_topic_score_codex":0.0037874652,"about_ca_topic_score_gemma":0.007064243,"teacher_disagreement_score":0.0037874652,"about_ca_system_score_codex":0.00025375857,"about_ca_system_score_gemma":0.00023757774,"threshold_uncertainty_score":0.0075308084},"labels":[],"label_agreement":null},{"id":"W2143906291","doi":"10.1088/0004-637x/767/2/131","title":"THE COMPARATIVE CHEMICAL EVOLUTION OF AN ISOLATED DWARF GALAXY: A VLT AND KECK SPECTROSCOPIC SURVEY OF WLM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Metallicity; Local Group; Dwarf galaxy; Galaxy; Astronomy; Stars; Large Magellanic Cloud; Irregular galaxy; Dwarf spheroidal galaxy; Interacting galaxy","score_opus":0.010686017070543728,"score_gpt":0.23330684156333106,"score_spread":0.22262082449278733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143906291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992362,0.000052151037,0.00004050294,0.0000071292443,5.5323477e-7,0.000001608735,0.00025840368,0.0000045991906,0.00039875854],"genre_scores_gemma":[0.99878305,0.000043368374,0.00012522598,0.000014751083,0.0000030187218,0.0000035554176,0.000756803,0.0000055880932,0.00026466436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998777,0.00000915159,0.000007556225,0.000052371324,0.000020614325,0.00003266979],"domain_scores_gemma":[0.99958867,0.000025392226,0.00015140449,0.00003328965,0.00004285324,0.00015829736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015373924,0.00014898245,0.00025557476,0.0019188265,0.00028780164,0.0005210777,0.00024277317,0.00018666843,0.0012451124],"category_scores_gemma":[0.00040186913,0.00010900372,0.00016288746,0.0009884378,0.0002536357,0.00039530676,0.00086531334,0.00015147967,0.0003894442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006308577,0.000031404765,0.9889903,0.000014426924,0.000034175715,0.00009388168,0.00036397038,0.00008282241,0.005289411,0.00009968686,0.00014587725,0.004790946],"study_design_scores_gemma":[0.0000012121635,0.000016616154,0.99939406,0.0000023917598,0.0000051592783,0.000070350885,0.00014597144,0.000075724,0.000093991155,0.000012403832,0.00018082607,0.0000013643624],"about_ca_topic_score_codex":0.007789936,"about_ca_topic_score_gemma":0.018823178,"teacher_disagreement_score":0.007789936,"about_ca_system_score_codex":0.00037116298,"about_ca_system_score_gemma":0.00012094775,"threshold_uncertainty_score":0.015489221},"labels":[],"label_agreement":null},{"id":"W2143979405","doi":"10.1088/0004-637x/716/1/198","title":"THE DISKMASS SURVEY. I. OVERVIEW","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":216,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Measure (data warehouse); Halo; Spiral galaxy; Tully–Fisher relation; Kinematics; Calibration; Stellar mass; Disc","score_opus":0.011752629137916665,"score_gpt":0.2352032456987351,"score_spread":0.22345061656081844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2143979405","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.022930812,0.02227352,0.010695246,0.002500035,0.0005368847,0.0010589793,0.86792225,0.0055637937,0.06651852],"genre_scores_gemma":[0.037720237,0.013788492,0.022927342,0.0012108539,0.0006919668,0.0013255567,0.88817614,0.0008518699,0.033307634],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9992582,0.00010429178,0.00008272582,0.00021242982,0.00024358218,0.00009875767],"domain_scores_gemma":[0.99838567,0.00010925412,0.00026034718,0.00030937197,0.00056090805,0.00037456187],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014276998,0.0014485478,0.00074850465,0.009417855,0.00050307513,0.0016691508,0.0020010523,0.00055900775,0.025199553],"category_scores_gemma":[0.0013978666,0.00048685115,0.0003350673,0.0085315,0.00026198968,0.001701759,0.0020789318,0.00055614667,0.036756363],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030005313,0.000119018485,0.10229765,0.0017363973,0.000109470275,0.00013317444,0.00027466705,0.00043312524,0.0027757606,0.0039052658,0.5945999,0.29331553],"study_design_scores_gemma":[0.000022339429,0.000031565472,0.06603607,0.00018869623,0.000020578278,0.0002042701,0.000118193486,0.00022130425,0.00043430418,0.001158203,0.9315486,0.000015982423],"about_ca_topic_score_codex":0.013965537,"about_ca_topic_score_gemma":0.01771302,"teacher_disagreement_score":0.025199553,"about_ca_system_score_codex":0.0010303918,"about_ca_system_score_gemma":0.0013224272,"threshold_uncertainty_score":0.084300935},"labels":[],"label_agreement":null},{"id":"W2144022483","doi":"10.1088/0004-637x/768/2/129","title":"MICROLENSING DISCOVERY OF A POPULATION OF VERY TIGHT, VERY LOW MASS BINARY BROWN DWARFS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Japan Society for the Promotion of Science; Science and Technology Facilities Council; Fédération Wallonie-Bruxelles; Chungbuk National University; Fonds National de la Recherche Luxembourg; Qatar National Research Fund; Qatar Foundation; Korea Research Council of Fundamental Science and Technology; Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture; Deutsche Forschungsgemeinschaft; Leverhulme Trust; California Institute of Technology; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Gravitational microlensing; Brown dwarf; Physics; Astrophysics; Low Mass; Astronomy; Binary number; Population; Stellar mass; Stars; Star formation","score_opus":0.007455050579949903,"score_gpt":0.20516246540067073,"score_spread":0.19770741482072082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144022483","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99705625,0.00039554652,0.00079826155,0.0000671366,0.000006169752,0.0000046510168,0.00008211679,0.000035347643,0.0015545817],"genre_scores_gemma":[0.99925107,0.00004914685,0.00036825353,0.00004809502,0.000008586059,0.0000016270241,0.00010872408,0.000002396934,0.00016207737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997409,0.000016374977,0.000011496803,0.00009617778,0.00008002076,0.000055092318],"domain_scores_gemma":[0.9994122,0.000095024305,0.00017600163,0.000049895716,0.000061938306,0.00020500265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003698737,0.00015737592,0.0002733086,0.0014407933,0.0006446673,0.0012119637,0.00038825223,0.0003927437,0.0007126409],"category_scores_gemma":[0.0008397968,0.00018437572,0.00008161407,0.0005471277,0.00056679896,0.00033471803,0.0011352634,0.0003607534,0.00014825462],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029277566,0.000079082565,0.77506405,0.00006203645,0.0000681317,0.0007783264,0.0008994878,0.00020893382,0.17593533,0.003226864,0.00069502654,0.04269002],"study_design_scores_gemma":[0.000015133478,0.00013909959,0.97554964,0.000010137334,0.000043376112,0.0025181512,0.00037896857,0.00096270605,0.016916832,0.001218419,0.0022253252,0.000022232536],"about_ca_topic_score_codex":0.002175647,"about_ca_topic_score_gemma":0.0027294597,"teacher_disagreement_score":0.002175647,"about_ca_system_score_codex":0.000544011,"about_ca_system_score_gemma":0.0001416293,"threshold_uncertainty_score":0.0043259263},"labels":[],"label_agreement":null},{"id":"W2144116455","doi":"10.1088/0004-637x/784/2/143","title":"A MEASUREMENT OF THE SECONDARY-CMB AND MILLIMETER-WAVE-FOREGROUND BISPECTRUM USING 800 deg<sup>2</sup>OF SOUTH POLE TELESCOPE DATA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; National Energy Research Scientific Computing Center; U.S. Department of Energy; McGill University; Gordon and Betty Moore Foundation; Office of Science; Canada Research Chairs; National Aeronautics and Space Administration; National Science Foundation","keywords":"Bispectrum; Physics; Cosmic microwave background; Astrophysics; South Pole Telescope; Spectral density; Multipole expansion; Amplitude; Telescope; Anisotropy; Optics; Statistics; Mathematics","score_opus":0.025999820857535556,"score_gpt":0.2187338533548648,"score_spread":0.19273403249732926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144116455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9633888,0.00014607915,0.0117132515,0.00009717717,0.000020856089,0.00006072934,0.013028782,0.0005587778,0.010985468],"genre_scores_gemma":[0.95706064,0.00014267043,0.018029025,0.00004909448,0.00005103689,0.00007253985,0.0226177,0.00012728834,0.0018500775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994773,0.000040415274,0.000020953416,0.00013943661,0.00023543184,0.00008646999],"domain_scores_gemma":[0.9986046,0.00021974945,0.0003949007,0.00026787905,0.00029304103,0.0002198444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003935236,0.00035458404,0.00025801995,0.0023191131,0.0002685786,0.000521691,0.00042936686,0.0003059151,0.0030676576],"category_scores_gemma":[0.0013514401,0.0002256987,0.00025091274,0.0020322497,0.00014532323,0.00042695508,0.00048732097,0.00030127369,0.0014377101],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005709022,0.00014507772,0.7976625,0.000117164156,0.00018757951,0.0001904161,0.0004008627,0.0016372752,0.099884786,0.0012262736,0.0045906194,0.09338648],"study_design_scores_gemma":[0.0000076093893,0.000022924432,0.9858272,0.0000037738205,0.000021954125,0.00012046715,0.000042250056,0.0024140917,0.0074234023,0.00012042638,0.0039850604,0.000010691823],"about_ca_topic_score_codex":0.0050314614,"about_ca_topic_score_gemma":0.013083543,"teacher_disagreement_score":0.0050314614,"about_ca_system_score_codex":0.0005232876,"about_ca_system_score_gemma":0.00017735019,"threshold_uncertainty_score":0.01026237},"labels":[],"label_agreement":null},{"id":"W2144118446","doi":"10.1086/509884","title":"Imbalanced Strong MHD Turbulence","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Cascade; Turbulence; Dissipation; Magnetohydrodynamics; Energy cascade; Amplitude; Mechanics; Wavenumber; Magnetohydrodynamic turbulence; Solar wind; Classical mechanics; Magnetic field; Quantum mechanics","score_opus":0.00647842486579417,"score_gpt":0.23859333736675808,"score_spread":0.23211491250096392,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144118446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7667526,0.00078010076,0.1631457,0.0021144785,0.0003590389,0.00013306223,0.000681009,0.00032256724,0.06571133],"genre_scores_gemma":[0.9929871,0.00012166515,0.0022431905,0.00007539089,0.00007316053,0.000040705178,0.00005514532,0.000010339239,0.00439336],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998765,0.000023273853,0.000006053124,0.000020463925,0.000043234508,0.00003041008],"domain_scores_gemma":[0.9998777,0.000015427113,0.000031325777,0.000015468891,0.00001760612,0.000042466312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015871458,0.00046878183,0.00041885438,0.00033243943,0.0005842402,0.0009399497,0.0008640334,0.0009287109,0.0019469173],"category_scores_gemma":[0.0005035976,0.00016994434,0.00042168403,0.00021955592,0.00094711763,0.0013419023,0.0013480149,0.00056459184,0.00024085268],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027518548,0.00012597612,0.0048389826,0.0001312374,0.00005325229,0.0012115294,0.00041622264,0.47645932,0.023923505,0.4859287,0.0023037372,0.004332309],"study_design_scores_gemma":[0.000054540225,0.00006396961,0.0011755388,0.000007512577,0.000010368732,0.00011995378,0.00006313402,0.9550654,0.00040924642,0.04137536,0.0016368882,0.000018158025],"about_ca_topic_score_codex":0.0027150991,"about_ca_topic_score_gemma":0.0011265315,"teacher_disagreement_score":0.0027150991,"about_ca_system_score_codex":0.0006738324,"about_ca_system_score_gemma":0.00039749756,"threshold_uncertainty_score":0.0065131187},"labels":[],"label_agreement":null},{"id":"W2144157858","doi":"10.1088/0004-637x/711/2/1185","title":"SPECTROSCOPIC CONFIRMATION OF THREE RED-SEQUENCE SELECTED GALAXY CLUSTERS AT<i>z</i>= 0.87, 1.16, AND 1.21 FROM THE SPARCS SURVEY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; University of Toronto","funders":"California Institute of Technology; W. M. Keck Foundation; Jet Propulsion Laboratory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Cluster (spacecraft); Galaxy cluster; Galaxy; Galaxy groups and clusters; Type-cD galaxy; Sample (material); Open cluster","score_opus":0.017242908750344135,"score_gpt":0.24215855504841613,"score_spread":0.22491564629807198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144157858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99878055,0.00004195999,0.00018536547,0.000021999147,0.00000558865,0.000010929644,0.00014175008,0.000015795784,0.000796105],"genre_scores_gemma":[0.9974172,0.00004284996,0.00103355,0.000046168658,0.000008893366,0.0000103925,0.0009641752,0.000007525535,0.00046914115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996487,0.000018934956,0.000028182507,0.00010480723,0.000108767344,0.00009069116],"domain_scores_gemma":[0.9986993,0.000098134966,0.00028502702,0.00011995549,0.00025745726,0.0005400384],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005078587,0.0003003631,0.00027996238,0.0011961733,0.0010581748,0.0007166103,0.00062498706,0.00033386552,0.0010692894],"category_scores_gemma":[0.00075459114,0.00025038436,0.00022133513,0.00039081095,0.0005378136,0.00025714346,0.0010886779,0.0004379861,0.00030211097],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020078145,0.0000749734,0.9313932,0.000027292359,0.000058116017,0.00057156605,0.00084397703,0.00029232088,0.05777257,0.00041487647,0.00047185356,0.007878458],"study_design_scores_gemma":[0.0000207797,0.00008801294,0.9880493,0.0000044714297,0.000034974888,0.00059469417,0.0002758812,0.00036343912,0.009181599,0.00006759045,0.0013047935,0.000014413252],"about_ca_topic_score_codex":0.011204113,"about_ca_topic_score_gemma":0.02993698,"teacher_disagreement_score":0.011204113,"about_ca_system_score_codex":0.0006097398,"about_ca_system_score_gemma":0.00049355184,"threshold_uncertainty_score":0.022277832},"labels":[],"label_agreement":null},{"id":"W2144191563","doi":"10.1088/0004-637x/814/2/132","title":"A SPATIALLY RESOLVED STUDY OF THE SYNCHROTRON EMISSION AND TITANIUM IN TYCHO’S SUPERNOVA REMNANT USING<i>NuSTAR</i>","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Space Telescope Science Institute; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Physics; Synchrotron; Astrophysics; Supernova; Supernova remnant; Titanium; Astronomy; Synchrotron radiation; Optics","score_opus":0.031193167583930065,"score_gpt":0.2601872663379811,"score_spread":0.22899409875405105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144191563","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991442,0.00007134951,0.0002437226,0.000005608322,0.0000010009913,0.0000023941648,0.00010796051,0.000012067681,0.00041169007],"genre_scores_gemma":[0.9978678,0.00007887943,0.0012372431,0.000011438748,0.000004928789,0.0000047305725,0.0005426401,0.000010209621,0.00024208476],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999944,0.000004467943,0.0000035063604,0.000018186553,0.000013744435,0.000016206706],"domain_scores_gemma":[0.999726,0.000029609275,0.00010179834,0.00004199462,0.00004641528,0.000054187596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001280834,0.0001622222,0.00017955125,0.0006305694,0.0003465386,0.0003337312,0.00022599676,0.0001481581,0.0005331859],"category_scores_gemma":[0.0002625981,0.00017501514,0.00025128262,0.0006570294,0.00019945813,0.00015799902,0.00041570712,0.00017590972,0.0001473653],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034317636,0.000060368548,0.58325917,0.00006528965,0.00016691643,0.00086115673,0.0008902404,0.0009513428,0.39967942,0.00021297061,0.00018515423,0.013324832],"study_design_scores_gemma":[0.0000053874132,0.00009019118,0.9891311,0.0000048950565,0.00003387896,0.00059252564,0.00019754951,0.0007782692,0.008417878,0.0000388991,0.0007022753,0.000007202812],"about_ca_topic_score_codex":0.0065420847,"about_ca_topic_score_gemma":0.01724054,"teacher_disagreement_score":0.0065420847,"about_ca_system_score_codex":0.00022284026,"about_ca_system_score_gemma":0.00013160304,"threshold_uncertainty_score":0.0130079985},"labels":[],"label_agreement":null},{"id":"W2144205038","doi":"10.1088/0004-637x/807/1/91","title":"RADIO TIMING AND OPTICAL PHOTOMETRY OF THE BLACK WIDOW SYSTEM PSR J1953+1846A IN THE GLOBULAR CLUSTER M71","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Aeronautics and Space Administration","keywords":"Millisecond pulsar; Pulsar; Globular cluster; Light curve; Binary pulsar; Photometry (optics); Pulsar planet; Orbital period; Neutron star","score_opus":0.019592564301233448,"score_gpt":0.3046629481286186,"score_spread":0.28507038382738514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144205038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995011,0.000041698706,0.0000594338,0.0000054038637,0.0000018831025,0.0000020076131,0.00009745892,0.000007747663,0.00028317556],"genre_scores_gemma":[0.9991161,0.000033985394,0.00022864561,0.0000066905895,0.0000057205216,0.0000020526447,0.00040899575,0.0000026814869,0.0001950336],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990857,0.0000054236243,0.000004112421,0.000020929914,0.000022342101,0.00003860553],"domain_scores_gemma":[0.9998173,0.000011527216,0.00006492125,0.00001732534,0.000029255601,0.00005973803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012280497,0.00015091899,0.00016932144,0.0010812506,0.00042583872,0.0002986991,0.00018174274,0.00021812785,0.00062119623],"category_scores_gemma":[0.00026898785,0.000085112755,0.00012119458,0.0006553131,0.00017178517,0.00012309877,0.00030558277,0.0001279363,0.00032067992],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004690091,0.00011158976,0.8541276,0.00005674926,0.000048711147,0.0012083504,0.000735643,0.0007141805,0.117001325,0.0002525469,0.0008000568,0.024474254],"study_design_scores_gemma":[0.000004378842,0.000075456,0.9970325,0.0000019929153,0.000009038952,0.00031075167,0.00010800546,0.00026849008,0.0016246765,0.000020653148,0.0005391417,0.000004886171],"about_ca_topic_score_codex":0.005332878,"about_ca_topic_score_gemma":0.008800438,"teacher_disagreement_score":0.005332878,"about_ca_system_score_codex":0.00028587694,"about_ca_system_score_gemma":0.00012155823,"threshold_uncertainty_score":0.010603666},"labels":[],"label_agreement":null},{"id":"W2144549738","doi":"10.1088/0004-637x/767/1/36","title":"A<i>HERSCHEL</i>AND APEX CENSUS OF THE REDDEST SOURCES IN ORION: SEARCHING FOR THE YOUNGEST PROTOSTARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":182,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"European Southern Observatory; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Protostar; Radiative transfer; Space observatory; Stars; Star formation; Young stellar object; Envelope (radar); Census","score_opus":0.014181380707217155,"score_gpt":0.24407283318259343,"score_spread":0.22989145247537626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144549738","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889608,0.0002626929,0.0002817394,0.000055821358,0.000004201733,0.000033880493,0.008571136,0.000071640236,0.0017580575],"genre_scores_gemma":[0.9245554,0.0005886689,0.0064392467,0.00013407091,0.00006763867,0.000109529894,0.06505586,0.00012671106,0.0029227869],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996124,0.000026647771,0.000025127216,0.000112850386,0.00012705279,0.000095948584],"domain_scores_gemma":[0.9987336,0.00010466795,0.0003673359,0.00020770654,0.00016568246,0.0004210326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052723486,0.0003486189,0.00037885038,0.003352765,0.00045944273,0.0008527113,0.00042438574,0.0002598369,0.0025238334],"category_scores_gemma":[0.000817167,0.00020029132,0.00033185518,0.0018266916,0.00020476113,0.00039618125,0.0015570653,0.00027076402,0.00098262],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009267266,0.00007201526,0.965683,0.000048937298,0.00006009307,0.00036165616,0.0004717657,0.0005241116,0.012712741,0.0003636904,0.003245845,0.016363462],"study_design_scores_gemma":[0.000012447585,0.000023187162,0.99350524,0.0000060850157,0.000013899347,0.00016875062,0.00010509318,0.0005519851,0.00087098597,0.00003986784,0.0046954276,0.0000069775097],"about_ca_topic_score_codex":0.011922007,"about_ca_topic_score_gemma":0.02529105,"teacher_disagreement_score":0.011922007,"about_ca_system_score_codex":0.00055517664,"about_ca_system_score_gemma":0.0006307837,"threshold_uncertainty_score":0.023705244},"labels":[],"label_agreement":null},{"id":"W2144728917","doi":"10.1088/0004-637x/748/2/123","title":"THE<i>HERSCHEL</i>REFERENCE SURVEY: DUST IN EARLY-TYPE GALAXIES AND ACROSS THE HUBBLE SEQUENCE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":202,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Virgo Cluster; Luminous infrared galaxy; Astronomy; Spiral galaxy; Photometry (optics); Elliptical galaxy; Stellar mass; Star formation; Stars","score_opus":0.025952663410637764,"score_gpt":0.2619663904747059,"score_spread":0.23601372706406812,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144728917","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.33229464,0.0054615615,0.0024503455,0.0056203613,0.00056625466,0.00015546296,0.615526,0.0022531918,0.035672177],"genre_scores_gemma":[0.5510221,0.0024677708,0.00685605,0.0030393433,0.0011734655,0.0001428151,0.40180746,0.0008449052,0.03264601],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970156,0.000018938901,0.000018347602,0.00007627815,0.000099846075,0.00008492053],"domain_scores_gemma":[0.99828786,0.00009317185,0.00054448267,0.00018450156,0.00033768607,0.0005522364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087540766,0.0005527823,0.0005631684,0.0049096667,0.0006077153,0.001153303,0.0009469404,0.001007073,0.0111151505],"category_scores_gemma":[0.0010877035,0.0002669557,0.00041826643,0.0048492257,0.00026066042,0.0008761224,0.0013672555,0.00056334154,0.005303945],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004551401,0.00015946795,0.531053,0.000351856,0.00023412188,0.00028327075,0.0005786957,0.001122277,0.012101763,0.0017498744,0.38199547,0.06991509],"study_design_scores_gemma":[0.000020984802,0.000020181367,0.96764773,0.00003063164,0.000027493867,0.000059234313,0.00008610959,0.00015504516,0.0006303106,0.0002065382,0.031101659,0.000014153845],"about_ca_topic_score_codex":0.08067701,"about_ca_topic_score_gemma":0.14501324,"teacher_disagreement_score":0.08067701,"about_ca_system_score_codex":0.0011555088,"about_ca_system_score_gemma":0.0012457881,"threshold_uncertainty_score":0.16041481},"labels":[],"label_agreement":null},{"id":"W2144772031","doi":"10.1088/0004-637x/786/1/43","title":"STATISTICAL AND SYSTEMATIC ERRORS IN THE MEASUREMENT OF WEAK-LENSING MINKOWSKI FUNCTIONALS: APPLICATION TO THE CANADA-FRANCE-HAWAII LENSING SURVEY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Weak gravitational lensing; Physics; Dark energy; Redshift; Astrophysics; Photometric redshift; Galaxy; Equation of state; Sigma; Cosmology; Omega; COSMIC cancer database; Observational error; Minkowski space; Gravitational lens; Gravitational lensing formalism; Astronomy; Statistics; Mathematical physics; Quantum mechanics; Mathematics","score_opus":0.012918643439713889,"score_gpt":0.2133951301871458,"score_spread":0.2004764867474319,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144772031","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98861897,0.00026950438,0.007225196,0.00015403889,0.000007636703,0.000024529098,0.0019575949,0.00014762046,0.0015947968],"genre_scores_gemma":[0.99364144,0.00009548922,0.004133911,0.000019909226,0.0000071210598,0.00001431902,0.0017880452,0.000023591236,0.0002762266],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99799734,0.00082803174,0.00011060789,0.0003512915,0.00060774613,0.00010500997],"domain_scores_gemma":[0.98651844,0.005802313,0.0024009985,0.0022223722,0.0026747065,0.00038118346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005330845,0.0005107087,0.00030286395,0.0023077158,0.00060998276,0.0009740119,0.0007027612,0.00027725298,0.0006339185],"category_scores_gemma":[0.020880915,0.00022426364,0.0003715315,0.0037019572,0.0007505836,0.0005148587,0.0010167166,0.0003047533,0.00010995413],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045200188,0.000013964385,0.96949446,0.000026439742,0.00019595551,0.00006844638,0.00035434312,0.011609005,0.0007531641,0.0021816513,0.00063426286,0.014623153],"study_design_scores_gemma":[0.00000629861,0.000022737959,0.9566086,0.000023028331,0.00004664543,0.00008512667,0.00027716887,0.03763892,0.0015341793,0.0013823959,0.0023317912,0.000042933196],"about_ca_topic_score_codex":0.36166808,"about_ca_topic_score_gemma":0.3262743,"teacher_disagreement_score":0.6383319,"about_ca_system_score_codex":0.00240617,"about_ca_system_score_gemma":0.0014157582,"threshold_uncertainty_score":0.71912587},"labels":[],"label_agreement":null},{"id":"W2144785544","doi":"10.1088/0004-637x/721/1/715","title":"REVERBERATION MAPPING MEASUREMENTS OF BLACK HOLE MASSES IN SIX LOCAL SEYFERT GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":359,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Reverberation mapping; Physics; Active galactic nucleus; Astrophysics; Supermassive black hole; Galaxy; Reverberation; Black hole (networking); Context (archaeology); Luminosity; Accretion (finance); Astronomy; Geology","score_opus":0.015181271201809586,"score_gpt":0.22415667106659032,"score_spread":0.20897539986478073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144785544","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999419,0.000023600085,0.0003028481,0.0000030762105,9.428122e-7,0.0000036380086,0.00007721746,0.000019208632,0.00015051707],"genre_scores_gemma":[0.99827003,0.000028417064,0.001020273,0.0000048897687,0.000006895067,0.0000062395075,0.00032918772,0.00000985379,0.0003241543],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998702,0.000021571963,0.0000069179587,0.000043213873,0.0000310194,0.000027153259],"domain_scores_gemma":[0.9993544,0.00010195468,0.00017474766,0.00010899873,0.0001257386,0.00013422105],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045335357,0.00031967473,0.00024642824,0.0013062087,0.00032754184,0.0003235614,0.00026337916,0.0002433906,0.0009074139],"category_scores_gemma":[0.00079118385,0.00018152296,0.0001871348,0.0004881658,0.00021708195,0.00024520716,0.00036496617,0.00020497153,0.0003706114],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065733556,0.000121224584,0.8455113,0.0000380562,0.00006750756,0.00030222978,0.0018641825,0.00065828697,0.1239121,0.00006360525,0.0001263721,0.026677772],"study_design_scores_gemma":[0.000005907566,0.00011973082,0.99418193,0.0000010796897,0.0000149612515,0.00011281057,0.000079903184,0.00034602356,0.004935573,0.000012716158,0.00018517199,0.000004247981],"about_ca_topic_score_codex":0.002874471,"about_ca_topic_score_gemma":0.007866909,"teacher_disagreement_score":0.002874471,"about_ca_system_score_codex":0.00021687694,"about_ca_system_score_gemma":0.000058400095,"threshold_uncertainty_score":0.005715549},"labels":[],"label_agreement":null},{"id":"W2144794357","doi":"10.1088/0004-637x/784/1/1","title":"SHOCKS AND STAR FORMATION IN STEPHAN'S QUINTET. I. GEMINI SPECTROSCOPY OF Hα-BRIGHT KNOTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Star formation; Galaxy; Redshift; Line (geometry); Emission spectrum; Spectroscopy; Spectral line; Astronomy; Geometry","score_opus":0.00497523198503433,"score_gpt":0.20878666279193134,"score_spread":0.203811430806897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144794357","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99968493,0.000022416274,0.000025348141,0.000008460584,3.5206304e-7,0.0000013265968,0.000022919538,0.000003469519,0.0002308876],"genre_scores_gemma":[0.9997693,0.00001165604,0.00005092354,0.0000048507472,0.000001002728,7.644958e-7,0.00006166322,0.0000013180511,0.00009858924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999355,0.000004420441,0.0000017838578,0.000020108308,0.000014562124,0.000023681607],"domain_scores_gemma":[0.9997832,0.000016584067,0.00007679512,0.00001744658,0.00001762838,0.000088423774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008768033,0.00017055536,0.00015433424,0.00065663125,0.0005046976,0.0003214914,0.0002943158,0.0002016084,0.001013196],"category_scores_gemma":[0.00022882324,0.00012373297,0.00009204847,0.0007081757,0.00030105404,0.00021179629,0.00062479026,0.00018705096,0.00011935364],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033087315,0.000063427244,0.91941047,0.000021736845,0.000033826986,0.0014980789,0.002185939,0.00047434523,0.065922745,0.00033862152,0.0002068251,0.009513179],"study_design_scores_gemma":[0.0000044575004,0.000058061716,0.9967006,0.0000016940091,0.0000063039975,0.00034059203,0.0003719898,0.0004755749,0.0014252777,0.0000817207,0.0005296256,0.0000040123496],"about_ca_topic_score_codex":0.010242157,"about_ca_topic_score_gemma":0.017013852,"teacher_disagreement_score":0.010242157,"about_ca_system_score_codex":0.00042355535,"about_ca_system_score_gemma":0.00011003552,"threshold_uncertainty_score":0.020365119},"labels":[],"label_agreement":null},{"id":"W2144960271","doi":"10.1088/0004-637x/773/2/181","title":"METAL ABUNDANCES, RADIAL VELOCITIES, AND OTHER PHYSICAL CHARACTERISTICS FOR THE RR LYRAE STARS IN THE<i>KEPLER</i>FIELD","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":147,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Research Canada; Camosun College","funders":"Science Mission Directorate; Magyar Tudományos Akadémia; Hungarian Scientific Research Fund; National Aeronautics and Space Administration; National Science Foundation","keywords":"RR Lyrae variable; Stars; Copernicus; Research council; Gamma-ray astronomy","score_opus":0.013189506792991324,"score_gpt":0.23011945284782556,"score_spread":0.21692994605483423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2144960271","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99912614,0.00009212924,0.000055538025,0.0000052651917,7.3965253e-7,0.000001757004,0.00021925698,0.0000058939463,0.0004933588],"genre_scores_gemma":[0.9984535,0.00007122516,0.00019709625,0.0000064775186,0.0000036240554,0.0000030836463,0.0008175737,0.000003410578,0.0004441279],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998925,0.000010535581,0.000016254597,0.00003580648,0.00002112707,0.00002385485],"domain_scores_gemma":[0.99941397,0.00010335112,0.00022775064,0.000057210185,0.00006897287,0.00012866793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026289996,0.00024092205,0.00019965334,0.0020270515,0.00034626416,0.00031207385,0.00020776004,0.000179395,0.0012939177],"category_scores_gemma":[0.00060821883,0.0001067355,0.00015886372,0.00067284034,0.0002825217,0.00030275685,0.00030722332,0.00016049086,0.0006818482],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019024656,0.000019799563,0.98774815,0.000012973744,0.000020836998,0.00012529508,0.00016642206,0.000121550926,0.005787404,0.000046008197,0.00009288241,0.005668458],"study_design_scores_gemma":[0.0000023831112,0.000057668265,0.9988218,0.0000012431519,0.000006061623,0.00028799154,0.000084332176,0.00007330331,0.00036849975,0.00001956901,0.00027507584,0.0000020557109],"about_ca_topic_score_codex":0.0017456914,"about_ca_topic_score_gemma":0.0022116937,"teacher_disagreement_score":0.0020270515,"about_ca_system_score_codex":0.0002680488,"about_ca_system_score_gemma":0.00007385568,"threshold_uncertainty_score":0.0043286085},"labels":[],"label_agreement":null},{"id":"W2145009246","doi":"10.1086/587682","title":"<i>Chandra</i>X‐Ray Observations of the 0.6 &lt;<i>z</i>&lt; 1.1 Red‐Sequence Cluster Survey Sample","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"Scaling; Cluster (spacecraft); Surface brightness; Galaxy cluster; Baryon; Luminosity; Spectral line; Brightness","score_opus":0.033611121098572116,"score_gpt":0.22876508203772614,"score_spread":0.19515396093915402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145009246","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99338806,0.00006791562,0.00014483678,0.000029314264,0.0000027238495,0.00001461808,0.0049373615,0.000052089155,0.0013631906],"genre_scores_gemma":[0.98284966,0.00013738143,0.001381721,0.00005122233,0.00002040482,0.000024474346,0.013996325,0.000026544261,0.0015123284],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998785,0.000011137627,0.0000097475595,0.000025003514,0.000034407814,0.000041115618],"domain_scores_gemma":[0.99941456,0.000038337763,0.0002066122,0.00007000792,0.00007286297,0.00019765583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025919135,0.00020945008,0.00022293036,0.002018351,0.0003659961,0.0004084015,0.00026810708,0.00010159224,0.0020780365],"category_scores_gemma":[0.0003845477,0.00018766406,0.00023520376,0.00091036526,0.0001417974,0.00018715997,0.0005503427,0.00022977032,0.0006694509],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002928484,0.00009210596,0.9644461,0.000047201665,0.00007827165,0.00015277464,0.00034375183,0.0006002395,0.017698677,0.00027246872,0.004775469,0.011200051],"study_design_scores_gemma":[0.0000060799953,0.000020514977,0.9978005,0.000002208388,0.000008719671,0.00010496233,0.00003955003,0.00014614106,0.0005952859,0.000013944724,0.0012583197,0.0000036726685],"about_ca_topic_score_codex":0.011391366,"about_ca_topic_score_gemma":0.022882467,"teacher_disagreement_score":0.011391366,"about_ca_system_score_codex":0.0002460186,"about_ca_system_score_gemma":0.00020813935,"threshold_uncertainty_score":0.022650123},"labels":[],"label_agreement":null},{"id":"W2145049475","doi":"10.1088/0004-637x/714/2/1170","title":"A SURVEY OF EXTRAGALACTIC FARADAY ROTATION AT HIGH GALACTIC LATITUDE: THE VERTICAL MAGNETIC FIELD OF THE MILKY WAY TOWARD THE GALACTIC POLES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Milky Way; Astrophysics; Faraday effect; Galactic Center; Galaxy; Astronomy; Magnetic field; Galactic halo; Telescope; Halo","score_opus":0.009398618777208961,"score_gpt":0.23659103324737893,"score_spread":0.22719241447016997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145049475","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991597,0.00017336753,0.00010036394,0.000012111046,8.8666195e-7,0.0000014720289,0.00016446841,0.0000053865533,0.0003823595],"genre_scores_gemma":[0.9985721,0.00022971896,0.0002635874,0.000013047707,0.00000806442,0.0000029704374,0.00064907275,0.0000035137696,0.00025789478],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998568,0.0000228249,0.000008415217,0.000042983695,0.000039576316,0.000029344445],"domain_scores_gemma":[0.9994155,0.000059131064,0.0002449125,0.00005674817,0.00009291761,0.00013078563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017524842,0.00018063342,0.00020282927,0.0011581647,0.00022536518,0.00038348016,0.000142736,0.00018545777,0.0004490138],"category_scores_gemma":[0.00050989765,0.00012164856,0.00014656372,0.00080605637,0.00019927222,0.00029086493,0.0004887671,0.00012467429,0.00022093032],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000065526496,0.000018584884,0.97654516,0.000041735788,0.00009046676,0.00014206939,0.00053195877,0.0001247205,0.010530229,0.00008144024,0.0002296592,0.011598341],"study_design_scores_gemma":[0.000001323106,0.000018595041,0.99904555,0.0000018786611,0.0000078564435,0.000089650326,0.000067715126,0.000029007684,0.00019185174,0.000008138088,0.00053716527,0.0000012145256],"about_ca_topic_score_codex":0.0042886985,"about_ca_topic_score_gemma":0.009448452,"teacher_disagreement_score":0.0042886985,"about_ca_system_score_codex":0.00017406867,"about_ca_system_score_gemma":0.00016884615,"threshold_uncertainty_score":0.008527458},"labels":[],"label_agreement":null},{"id":"W2145059216","doi":"10.1086/508019","title":"The Intrinsic Size of Sagittarius A* from 0.35 to 6 cm","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":176,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Sagittarius A*; Scattering; Physics; Wavelength; Schwarzschild radius; Astrophysics; Lambda; Optics; Stars; Galactic Center","score_opus":0.006807158967275441,"score_gpt":0.21093004621538775,"score_spread":0.2041228872481123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145059216","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906233,0.0004514446,0.0027776023,0.00011309117,0.000014285399,0.0000064919172,0.0011187014,0.00046169915,0.0044334135],"genre_scores_gemma":[0.9960913,0.000080953294,0.0019709435,0.00005084591,0.00002384921,0.0000058215815,0.00149691,0.00003463665,0.00024457858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985814,0.000011647277,0.000005613492,0.000068772075,0.000034007913,0.000021892796],"domain_scores_gemma":[0.9995198,0.000058820122,0.00015105413,0.0000668181,0.00008845884,0.000114997165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016311608,0.00020848752,0.00016201723,0.000833525,0.00029099916,0.00044009983,0.00039448857,0.00024150664,0.000925131],"category_scores_gemma":[0.0003780235,0.00023348132,0.00027443716,0.00040461167,0.00023820146,0.00041665553,0.0005187078,0.00033679575,0.00034880688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037903187,0.0000715846,0.60525167,0.0001188699,0.00020716843,0.00028718315,0.00055023446,0.0024870252,0.34245604,0.0013508854,0.0023886135,0.04445167],"study_design_scores_gemma":[0.000008529651,0.00006934548,0.9854402,0.000006387853,0.000034816556,0.0002604482,0.000051056326,0.002380492,0.00762409,0.00042944375,0.0036756087,0.000019544796],"about_ca_topic_score_codex":0.002381912,"about_ca_topic_score_gemma":0.0050739935,"teacher_disagreement_score":0.002381912,"about_ca_system_score_codex":0.00036464952,"about_ca_system_score_gemma":0.00012511684,"threshold_uncertainty_score":0.0047361255},"labels":[],"label_agreement":null},{"id":"W2145100347","doi":"10.1086/312789","title":"Measuring the Ionization of O Star Winds","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Metallicity; Stars; Ionization; O-type star; Spectral line; Galaxy; Astronomy; Supergiant; Ion","score_opus":0.01378610711575259,"score_gpt":0.2076949460120266,"score_spread":0.193908838896274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145100347","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990435,0.000030935138,0.00020075537,0.000002743307,7.683262e-7,0.000001973399,0.0001367639,0.000009920474,0.00057266676],"genre_scores_gemma":[0.9988564,0.00004773466,0.00040845232,0.0000053739914,0.0000016671935,0.0000017919225,0.0005442761,0.0000053994613,0.00012893435],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999198,0.0000071873533,0.0000032955659,0.000027068505,0.000021812597,0.000020848809],"domain_scores_gemma":[0.999858,0.000023584013,0.000038915623,0.0000102011845,0.000030314546,0.000039012906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008583237,0.00020878951,0.00019071659,0.00055576005,0.0002573399,0.0002951878,0.00012491061,0.00023263934,0.00048606843],"category_scores_gemma":[0.0003555579,0.00010730064,0.00012281445,0.00039300794,0.00011422341,0.00021884468,0.00023904166,0.00012676229,0.00022125579],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002566051,0.00004287271,0.9149853,0.000026779671,0.00008451341,0.0001896461,0.00018363452,0.0022261043,0.06840267,0.0001725819,0.00021341791,0.013215779],"study_design_scores_gemma":[0.000007500883,0.00009855904,0.9880949,0.000004270354,0.000018714236,0.00013950671,0.00011685705,0.0050387476,0.0058114748,0.00012790409,0.0005329248,0.0000086912905],"about_ca_topic_score_codex":0.0049981517,"about_ca_topic_score_gemma":0.0075104674,"teacher_disagreement_score":0.0049981517,"about_ca_system_score_codex":0.00019394557,"about_ca_system_score_gemma":0.000112552516,"threshold_uncertainty_score":0.009938121},"labels":[],"label_agreement":null},{"id":"W2145157017","doi":"10.1088/0004-637x/761/1/46","title":"THE DISCOVERY OF HD 37605<i>c</i>AND A DISPOSITIVE NULL DETECTION OF TRANSITS OF HD 37605<i>b</i>","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Ephemeris; Transit (satellite); Photometry (optics); Radial velocity; Exoplanet; Planet; Light curve; Jovian","score_opus":0.006159324883878141,"score_gpt":0.20456274155012336,"score_spread":0.19840341666624522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145157017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99283314,0.00025562177,0.00039063705,0.00011035049,0.00007108685,0.000015830323,0.0011095114,0.00008955164,0.0051241997],"genre_scores_gemma":[0.99721754,0.000046849444,0.00047692418,0.00011059127,0.000022992082,0.0000049049518,0.0014394694,0.00001372085,0.0006670095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967873,0.0000078943,0.000017555038,0.000119964854,0.000086596185,0.00008932256],"domain_scores_gemma":[0.9994555,0.000025653255,0.000128228,0.00008462399,0.000073165385,0.00023289547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019380156,0.00029092925,0.00028180022,0.001002065,0.0010400945,0.00058033917,0.00035955303,0.0007454576,0.0016176793],"category_scores_gemma":[0.0004833943,0.0001781077,0.00033019835,0.0007014234,0.0006466241,0.00024809098,0.0009624386,0.00043425776,0.0006925572],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007415288,0.00014290323,0.5806276,0.0002229585,0.0001519563,0.008470524,0.0016300983,0.0002621401,0.37531176,0.0026440325,0.0042700106,0.025524465],"study_design_scores_gemma":[0.000011390196,0.0001742336,0.96338207,0.000020610054,0.00005207881,0.0064106835,0.00029968258,0.00021070127,0.01722576,0.00023457054,0.011951934,0.000026322528],"about_ca_topic_score_codex":0.014107066,"about_ca_topic_score_gemma":0.017717883,"teacher_disagreement_score":0.014107066,"about_ca_system_score_codex":0.00049379416,"about_ca_system_score_gemma":0.00048871705,"threshold_uncertainty_score":0.028049946},"labels":[],"label_agreement":null},{"id":"W2145185355","doi":"10.1088/0004-637x/789/1/15","title":"A MAP OF DUST REDDENING TO 4.5 kpc FROM Pan-STARRS1","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Centre National de la Recherche Scientifique; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Queen's University; Johns Hopkins University; FAS Division of Science, Harvard University; Queen's University Belfast; National Aeronautics and Space Administration; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Sky; Dust lane; Cosmic dust; Extinction (optical mineralogy); Line (geometry); Milky Way","score_opus":0.009920534008751815,"score_gpt":0.21930518706999372,"score_spread":0.2093846530612419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145185355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9409344,0.0007845662,0.0039108447,0.0002233518,0.00004184467,0.00003871328,0.026104094,0.0013748325,0.026587276],"genre_scores_gemma":[0.9591784,0.0005337081,0.009135102,0.000047662783,0.00007163156,0.000027868033,0.026446646,0.00017426991,0.0043847905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998578,0.00000926673,0.0000051276425,0.000042962834,0.000061285195,0.000023614322],"domain_scores_gemma":[0.9996166,0.00003226963,0.00011888277,0.000049456765,0.000117866184,0.000064842505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013146557,0.00030198312,0.00020514651,0.0014791017,0.00027481443,0.00048138323,0.00024471973,0.00028193297,0.005054518],"category_scores_gemma":[0.00045701457,0.00015547956,0.00031064072,0.001119944,0.00012656639,0.00031398085,0.00044492717,0.00036475816,0.0017781301],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012044501,0.00020950317,0.60360575,0.0008807031,0.0005491881,0.0015816188,0.0017952948,0.022285318,0.1385375,0.003537555,0.0387559,0.18705729],"study_design_scores_gemma":[0.00002805561,0.00007183558,0.9650141,0.000025347172,0.000038697952,0.00038296473,0.00013487297,0.0039889007,0.004192989,0.00036045717,0.025740331,0.000021472677],"about_ca_topic_score_codex":0.0075366013,"about_ca_topic_score_gemma":0.007887151,"teacher_disagreement_score":0.0075366013,"about_ca_system_score_codex":0.00036337855,"about_ca_system_score_gemma":0.0002485171,"threshold_uncertainty_score":0.016909003},"labels":[],"label_agreement":null},{"id":"W2145265132","doi":"10.1086/323375","title":"Magnetic Fields in Star‐forming Molecular Clouds. II. The Depolarization Effect in the OMC‐3 Filament of Orion A","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McMaster University","funders":"","keywords":"Protein filament; Polarization (electrochemistry); Physics; James Clerk Maxwell Telescope; Polarimeter; Astrophysics; Magnetic field; Depolarization; Molecular cloud; Excitation; Telescope; Polarimetry; Geometry; Star formation; Optics; Galaxy; Scattering; Stars; Materials science; Chemistry","score_opus":0.005241688551303263,"score_gpt":0.22458210965245887,"score_spread":0.2193404211011556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145265132","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989293,0.00008929297,0.0001554374,0.000027320246,0.0000018540986,0.0000020362163,0.000061953746,0.000009168731,0.000723587],"genre_scores_gemma":[0.9997149,0.000037954083,0.00009757008,0.000004890233,0.0000040008117,0.0000011627025,0.00006378544,0.0000016327032,0.00007396482],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996746,0.0000040814593,0.0000014016271,0.0000050784706,0.000007107284,0.000014845564],"domain_scores_gemma":[0.99976283,0.000044965294,0.00010369152,0.00001326973,0.000033246582,0.000042050153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000062041916,0.00009119393,0.0000900893,0.00036825598,0.00027892995,0.00024161764,0.00015136879,0.00017433045,0.00040156738],"category_scores_gemma":[0.00044036272,0.00008060587,0.000073093026,0.00038296543,0.00023644333,0.00011695145,0.00022463495,0.00014920978,0.00008198286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010187564,0.00009763221,0.53963166,0.00014708938,0.000060113278,0.0017278119,0.00058878073,0.008423281,0.41859153,0.0030861355,0.0007277117,0.025899464],"study_design_scores_gemma":[0.000046424437,0.00008830427,0.9798884,0.000013191415,0.000026588523,0.0003965396,0.00014818774,0.00521962,0.012360691,0.0008321503,0.0009706863,0.000009217543],"about_ca_topic_score_codex":0.003934404,"about_ca_topic_score_gemma":0.002937287,"teacher_disagreement_score":0.003934404,"about_ca_system_score_codex":0.00036271938,"about_ca_system_score_gemma":0.00010110573,"threshold_uncertainty_score":0.00782305},"labels":[],"label_agreement":null},{"id":"W2145277944","doi":"10.1088/0004-637x/785/2/159","title":"SUBSTELLAR OBJECTS IN NEARBY YOUNG CLUSTERS (SONYC). VIII. SUBSTELLAR POPULATION IN LUPUS 3","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Systemic lupus erythematosus; Stellar classification; Population; Brown dwarf; Line (geometry); Type (biology); Spectral resolution","score_opus":0.0067726292870356804,"score_gpt":0.22036366192677334,"score_spread":0.21359103263973767,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145277944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99935716,0.00012779338,0.00012177092,0.000005609935,0.0000016453605,0.00000555759,0.00013968375,0.0000093749595,0.00023139243],"genre_scores_gemma":[0.9988337,0.00006172649,0.0003130643,0.0000065285853,0.0000057651496,0.000005393292,0.00063171284,0.0000024178908,0.00013967599],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985206,0.000011698636,0.000014717944,0.000041139712,0.000029538207,0.00005085229],"domain_scores_gemma":[0.99924505,0.000054335665,0.0003008892,0.000051055027,0.00007084369,0.00027781934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024074844,0.00015590058,0.00023325835,0.0014453455,0.0005792961,0.00045084755,0.00028295032,0.00019287596,0.001035361],"category_scores_gemma":[0.00036087752,0.000092919094,0.00026369348,0.0009097444,0.00029420725,0.00024409128,0.00068729743,0.00017171245,0.0002151957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011856791,0.000020250869,0.98897016,0.00001205705,0.000014306091,0.00023969587,0.00019389312,0.00007182268,0.005976651,0.00006130718,0.00012218452,0.004199104],"study_design_scores_gemma":[0.0000030474407,0.000034567303,0.9984855,0.00000191498,0.0000077425375,0.00041485886,0.0001255998,0.0001725241,0.00041054285,0.000032865155,0.00030880095,0.0000020475086],"about_ca_topic_score_codex":0.006607795,"about_ca_topic_score_gemma":0.009303638,"teacher_disagreement_score":0.006607795,"about_ca_system_score_codex":0.00040576718,"about_ca_system_score_gemma":0.00021880795,"threshold_uncertainty_score":0.013138652},"labels":[],"label_agreement":null},{"id":"W2145761433","doi":"10.1086/375509","title":"A Fast Gridded Method for the Estimation of the Power Spectrum of the Cosmic Microwave Background from Interferometer Data with Application to the Cosmic Background Imager","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Physics; Interferometry; Estimator; Spectral density; COSMIC cancer database; Aperture (computer memory); Noise (video); Optics; Astrophysics; Computer science; Acoustics; Anisotropy; Statistics; Mathematics; Telecommunications","score_opus":0.015017608485096102,"score_gpt":0.2811916325646566,"score_spread":0.26617402407956053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145761433","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0026851944,0.0001096123,0.99600345,0.000023052915,0.000035805166,0.000029623177,0.00027887552,0.0006181863,0.00021627119],"genre_scores_gemma":[0.0126961125,0.00007354184,0.98562604,0.00001720547,0.000018932229,0.00015388292,0.0007766541,0.00014703326,0.00049065246],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993173,0.00024787596,0.000045952518,0.00013261558,0.00022452,0.00003164291],"domain_scores_gemma":[0.9982326,0.00073495443,0.00012917051,0.00044895554,0.00041976842,0.000034500223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014712233,0.0006515566,0.00056698866,0.0017119348,0.00049551943,0.0008118137,0.0011743137,0.0005074051,0.003338184],"category_scores_gemma":[0.0057879323,0.00066995097,0.0007167694,0.0019190129,0.0004195507,0.00092187355,0.0010355953,0.0007844828,0.0017071262],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018609049,0.00009534813,0.009429236,0.0002816896,0.00036037207,0.00020276361,0.0001704709,0.13178657,0.02410209,0.0261283,0.0074242945,0.7998328],"study_design_scores_gemma":[0.00009981639,0.00008316534,0.009254806,0.000044245084,0.00006153863,0.0003769403,0.000042229065,0.93517005,0.010126087,0.021067888,0.023582695,0.0000905209],"about_ca_topic_score_codex":0.004754988,"about_ca_topic_score_gemma":0.007980086,"teacher_disagreement_score":0.004754988,"about_ca_system_score_codex":0.00041385368,"about_ca_system_score_gemma":0.0011368181,"threshold_uncertainty_score":0.011167347},"labels":[],"label_agreement":null},{"id":"W2145927470","doi":"10.1088/0004-637x/785/1/81","title":"ERRATUM: “ON THE KINEMATIC SEPARATION OF FIELD AND CLUSTER STARS ACROSS THE BULGE GLOBULAR NGC 6528” (2014, ApJ, 782, 50)","year":2014,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Bulge; Astrophysics; Stars; Kinematics; Astronomy; Classical mechanics","score_opus":0.010837471114457861,"score_gpt":0.2931267177173303,"score_spread":0.2822892466028724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145927470","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00069983635,0.00082549086,0.00036466727,0.0449733,0.93786514,0.000026802843,0.004343063,0.00047135545,0.010430252],"genre_scores_gemma":[0.019266479,0.0059414245,0.0039288304,0.11096116,0.22757085,0.000191223,0.021898806,0.002331444,0.6079098],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9980732,0.00014178499,0.00035014597,0.00031341566,0.0009211939,0.00020027216],"domain_scores_gemma":[0.98978233,0.0013137424,0.00069757696,0.0006789571,0.006942592,0.0005847927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015487574,0.002042584,0.0015901589,0.0038640758,0.004622365,0.0036418233,0.0030312352,0.0045031034,0.05157216],"category_scores_gemma":[0.017818246,0.0010913543,0.0013914667,0.002594981,0.0018185629,0.0028384875,0.0025700366,0.006688579,0.043222114],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003362044,0.00000862896,0.00013410918,0.000035155845,0.0000059270465,0.00007937164,0.000011542971,0.0000318175,0.000059939484,0.0003007674,0.9972806,0.002018536],"study_design_scores_gemma":[0.000059798134,0.000051349907,0.006879813,0.0002912846,0.00006047094,0.00023848757,0.00019832687,0.00023100022,0.00067634915,0.001877757,0.9893652,0.000070147915],"about_ca_topic_score_codex":0.048085164,"about_ca_topic_score_gemma":0.054416623,"teacher_disagreement_score":0.05157216,"about_ca_system_score_codex":0.003996839,"about_ca_system_score_gemma":0.006110826,"threshold_uncertainty_score":0.17252606},"labels":[],"label_agreement":null},{"id":"W2145948568","doi":"10.1088/0004-637x/781/1/35","title":"STATISTICAL SEARCHES FOR MICROLENSING EVENTS IN LARGE, NON-UNIFORMLY SAMPLED TIME-DOMAIN SURVEYS: A TEST USING PALOMAR TRANSIENT FACTORY DATA","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Weizmann Institute of Science; University of Oxford; York University; National Energy Research Scientific Computing Center; Carnegie Mellon University; University of Arizona; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory","keywords":"Gravitational microlensing; Physics; Light curve; Astrophysics; Photometry (optics); Event (particle physics); Sky; Galaxy; Stars","score_opus":0.03956753730655245,"score_gpt":0.28851682526026706,"score_spread":0.24894928795371463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145948568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98774624,0.00021395544,0.010842207,0.00026609647,0.000024491834,0.00008646618,0.00017432684,0.00014259425,0.0005035586],"genre_scores_gemma":[0.9925862,0.000050121187,0.0066122753,0.000093174065,0.000039721297,0.000031210533,0.00043087278,0.0000344421,0.00012186448],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.97347564,0.014124133,0.0023118411,0.004795264,0.0040552756,0.0012378157],"domain_scores_gemma":[0.43782166,0.5116776,0.024807991,0.015962407,0.0046698847,0.0050604558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.06090794,0.00081792386,0.0013448872,0.0031407212,0.0016950956,0.0024971447,0.0036529778,0.002718651,0.001455672],"category_scores_gemma":[0.14765067,0.000539118,0.002648011,0.0025267787,0.00532625,0.0042865467,0.0023588156,0.0015540725,0.00029724458],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.006356123,0.0008523657,0.8776672,0.00023551063,0.0019425561,0.0011848477,0.0009537099,0.07274135,0.0077858097,0.0058172103,0.0012053597,0.023257932],"study_design_scores_gemma":[0.0007445065,0.0046416554,0.35139254,0.00008972873,0.0005981137,0.0021466585,0.0022957576,0.6204793,0.010321329,0.0059458334,0.0011729733,0.00017169763],"about_ca_topic_score_codex":0.0026600435,"about_ca_topic_score_gemma":0.0017542312,"teacher_disagreement_score":0.06090794,"about_ca_system_score_codex":0.0012840146,"about_ca_system_score_gemma":0.0012748672,"threshold_uncertainty_score":0.32211584},"labels":[],"label_agreement":null},{"id":"W2145955890","doi":"10.1088/0004-637x/713/2/959","title":"PROPERTIES OF GALACTIC CIRRUS CLOUDS OBSERVED BY BOOMERANG","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cirrus; Physics; Spectral index; Astrophysics; Astronomy; Microwave; Wavelength; Emissivity; Cosmic dust; Spectral line; Atmospheric sciences; Optics","score_opus":0.016520086289245093,"score_gpt":0.21022762801239275,"score_spread":0.19370754172314766,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2145955890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843436,0.000100964,0.00017898079,0.000014912299,0.0000016887498,0.000002975982,0.00038189595,0.000027740378,0.00085647695],"genre_scores_gemma":[0.998638,0.0000537952,0.00026757398,0.000011425523,0.0000036257309,0.0000022953304,0.00089013175,0.00001382288,0.00011938959],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998621,0.000012892263,0.0000042614997,0.000045557164,0.000035494508,0.00003967629],"domain_scores_gemma":[0.9997279,0.00003288901,0.000089500565,0.00003576755,0.0000558617,0.000057981044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016511629,0.0002486951,0.0002457975,0.0012104587,0.00037313023,0.0004871854,0.00022779274,0.00019936629,0.000398549],"category_scores_gemma":[0.00038534275,0.00015708987,0.00019781663,0.0010609613,0.00025755123,0.0002768185,0.0002941646,0.00017575127,0.00020909033],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028739238,0.000046452544,0.93886864,0.000044507004,0.0001515853,0.00034292013,0.0007019257,0.0012530447,0.04733045,0.00017907967,0.00087775744,0.009916105],"study_design_scores_gemma":[0.0000030000376,0.000012220285,0.9971706,0.000002437353,0.000016854554,0.00008692317,0.00006273171,0.00073305797,0.0012209412,0.000016136284,0.0006688601,0.0000061258925],"about_ca_topic_score_codex":0.014492617,"about_ca_topic_score_gemma":0.023264458,"teacher_disagreement_score":0.014492617,"about_ca_system_score_codex":0.00033897444,"about_ca_system_score_gemma":0.00009703542,"threshold_uncertainty_score":0.028816521},"labels":[],"label_agreement":null},{"id":"W2146081406","doi":"10.1088/0004-637x/769/1/77","title":"MOA-2010-BLG-311: A PLANETARY CANDIDATE BELOW THE THRESHOLD OF RELIABLE DETECTION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"National Research Foundation of Korea; California Institute of Technology; European Commission; Qatar National Research Fund; Korea Research Council of Fundamental Science and Technology; Qatar Foundation; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Space Telescope Science Institute; Alfred P. Sloan Foundation; National Geographic Society; National Science Foundation","keywords":"Gravitational microlensing; Physics; Planet; Planetary system; Astrophysics; Event (particle physics); Lens (geology); Magnification; Astronomy; Stars; Optics","score_opus":0.00808162899290804,"score_gpt":0.1971085545147486,"score_spread":0.18902692552184056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146081406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9011039,0.0011081351,0.0031728304,0.004106408,0.00046678766,0.00008955446,0.0025128901,0.0006337164,0.08680571],"genre_scores_gemma":[0.98547703,0.000089245485,0.0020832554,0.000698846,0.00007210893,0.000014989534,0.0018252556,0.00007087963,0.00966848],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984896,0.000011865953,0.00000458087,0.000045348803,0.000034739176,0.00005460681],"domain_scores_gemma":[0.9994106,0.000050730418,0.00009326214,0.000054091517,0.000097528755,0.0002937159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024887847,0.00022021274,0.0002434261,0.0009012775,0.001689154,0.0010028353,0.00033509638,0.0012260829,0.010821001],"category_scores_gemma":[0.00077461626,0.00010430101,0.00018338651,0.0005591313,0.00045252914,0.00044656324,0.0008551035,0.0006362158,0.003131196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012010125,0.00032527922,0.6811387,0.00035731407,0.000109729655,0.014054444,0.0014435576,0.0006679148,0.098525554,0.018011792,0.043457486,0.14070724],"study_design_scores_gemma":[0.000059584898,0.00035259733,0.7812743,0.00012554393,0.00005751702,0.018830895,0.0014845822,0.0022126266,0.008444443,0.0070089293,0.18010236,0.00004665481],"about_ca_topic_score_codex":0.0039920984,"about_ca_topic_score_gemma":0.008138859,"teacher_disagreement_score":0.010821001,"about_ca_system_score_codex":0.00046880776,"about_ca_system_score_gemma":0.00052117853,"threshold_uncertainty_score":0.036199927},"labels":[],"label_agreement":null},{"id":"W2146124831","doi":"10.1086/508768","title":"A Search for Neutrinos from the Solar<i>hep</i>Reaction and the Diffuse Supernova Neutrino Background with the Sudbury Neutrino Observatory","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; University of Guelph; Queen's University; TRIUMF; Carleton University; Laurentian University","funders":"","keywords":"Neutrino; Solar neutrino; Supernova; Physics; Neutrino astronomy; Neutrino detector; Solar neutrino problem; Observatory; Measurements of neutrino speed; Astrophysics; Cosmic neutrino background; Electron neutrino; Astronomy; Neutrino oscillation; Particle physics","score_opus":0.024620815429817203,"score_gpt":0.2608476927051762,"score_spread":0.23622687727535902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146124831","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9863517,0.0021131283,0.0038627444,0.00030376148,0.000031843505,0.00005102544,0.0010951526,0.00008895482,0.0061016455],"genre_scores_gemma":[0.98702335,0.00078583416,0.00876035,0.0001312368,0.000074382944,0.00002473323,0.0019588096,0.000017932975,0.0012233047],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999276,0.00010305342,0.000029441171,0.00021098113,0.00024230574,0.0001382639],"domain_scores_gemma":[0.99873847,0.00017847274,0.00041606915,0.00012396801,0.0001531785,0.0003897731],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014425912,0.0007561888,0.00060321274,0.0017155323,0.0012272133,0.0013274292,0.00060505903,0.00045742185,0.0015865179],"category_scores_gemma":[0.0014237338,0.0004597654,0.00052187697,0.0013202438,0.0004949334,0.0006356264,0.0016880063,0.000817812,0.00022107128],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017234777,0.00021084727,0.7556773,0.00015497208,0.00055733294,0.001734073,0.00039626757,0.0010132334,0.17219204,0.0035141548,0.0016524935,0.061173823],"study_design_scores_gemma":[0.00020466931,0.00095830526,0.92117286,0.00007895643,0.00025719535,0.0027699007,0.00027344903,0.0049371333,0.053776182,0.0022507133,0.0132347755,0.00008581754],"about_ca_topic_score_codex":0.009553604,"about_ca_topic_score_gemma":0.015780643,"teacher_disagreement_score":0.009553604,"about_ca_system_score_codex":0.0006715383,"about_ca_system_score_gemma":0.0008174073,"threshold_uncertainty_score":0.018996},"labels":[],"label_agreement":null},{"id":"W2146270359","doi":"10.1086/425264","title":"Quiescent Dense Gas in Protostellar Clusters: The Ophiuchus A Core","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Astrophysics; Physics; Protostar; Maxima; Full width at half maximum; Line (geometry); Star formation; Galaxy; Optics; Geometry","score_opus":0.016021295986451602,"score_gpt":0.24944580748013315,"score_spread":0.23342451149368154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146270359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989475,0.00044415484,0.00009760454,0.0003933313,0.00010032066,0.000021030599,0.00033210445,0.000040667222,0.0090957405],"genre_scores_gemma":[0.99476516,0.00017739828,0.00006806772,0.00005581233,0.0001513886,0.000004762856,0.0003188142,0.000013025675,0.00444552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984217,0.000017450338,0.000010162765,0.00003370756,0.000055324148,0.00004120342],"domain_scores_gemma":[0.9962328,0.00049468083,0.0004619987,0.00015994853,0.0011418426,0.0015087237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033661164,0.00010574714,0.00025045907,0.0008859391,0.0008619612,0.0012358568,0.0004205133,0.00054802955,0.011088583],"category_scores_gemma":[0.0031603994,0.00013117194,0.00006286276,0.00059845916,0.0005499363,0.00069185597,0.00064959977,0.00018482121,0.0014687617],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0045963004,0.0004612772,0.805453,0.00038983513,0.00006416169,0.0037251753,0.00191276,0.001028092,0.06503796,0.006583483,0.035460316,0.07528758],"study_design_scores_gemma":[0.000105674815,0.00023619423,0.9841499,0.000020685753,0.000017170825,0.0005428901,0.00072017376,0.0009747413,0.003025566,0.0018154201,0.008377526,0.000014064735],"about_ca_topic_score_codex":0.0048509818,"about_ca_topic_score_gemma":0.0046895524,"teacher_disagreement_score":0.011088583,"about_ca_system_score_codex":0.00039923558,"about_ca_system_score_gemma":0.0007251681,"threshold_uncertainty_score":0.03709501},"labels":[],"label_agreement":null},{"id":"W2146337602","doi":"10.1086/421770","title":"On the O<scp>ii</scp>Ground Configuration Energy Levels","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Measure (data warehouse); Term (time); Orion Nebula; Spectroscopy; Energy (signal processing); Planetary nebula; Nebula; Ground state","score_opus":0.01977662690343466,"score_gpt":0.2604749666740975,"score_spread":0.24069833977066282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146337602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9452059,0.00033384742,0.02107868,0.00017997218,0.000017960176,0.000013143842,0.0004992731,0.0002457712,0.03242547],"genre_scores_gemma":[0.99475527,0.000097697826,0.004185893,0.00004652463,0.0000074988607,0.00001064039,0.00027184733,0.000039749786,0.00058492296],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981004,0.00001722912,0.000005670735,0.000050184975,0.00006713699,0.000049755414],"domain_scores_gemma":[0.999681,0.00009952062,0.000079539466,0.000066968336,0.00004666404,0.000026335707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024985804,0.00040774528,0.00017142731,0.001525888,0.0005695177,0.00056465995,0.0005177359,0.0003376757,0.0048139975],"category_scores_gemma":[0.00062148017,0.00019317854,0.00019895515,0.0013537465,0.0007296476,0.00061043695,0.00066728523,0.00055048306,0.0006933318],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087780756,0.00017490568,0.1365656,0.00026862527,0.00015344171,0.0011540919,0.0009207635,0.028999802,0.54757845,0.12338395,0.0034651577,0.1564574],"study_design_scores_gemma":[0.000103617625,0.00028361016,0.50560606,0.00020190995,0.000105392806,0.00097298226,0.0007665498,0.11218845,0.20475402,0.15743014,0.01744477,0.00014238869],"about_ca_topic_score_codex":0.0019172033,"about_ca_topic_score_gemma":0.00319481,"teacher_disagreement_score":0.0048139975,"about_ca_system_score_codex":0.00040926342,"about_ca_system_score_gemma":0.00014894779,"threshold_uncertainty_score":0.01610446},"labels":[],"label_agreement":null},{"id":"W2146602332","doi":"10.1088/0004-637x/705/2/1433","title":"INTERACTING GALAXIES IN THE A901/902 SUPERCLUSTER WITH STAGES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Space Telescope Science Institute; Deutsche Forschungsgemeinschaft; Austrian Science Fund; National Aeronautics and Space Administration; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"Supercluster (genetic); Galaxy merger; Physics; Astrophysics; Galaxy; Galaxy cluster; Merge (version control); Cluster (spacecraft); Velocity dispersion; RADIUS; Astronomy; Galaxy formation and evolution; Computer science; Information retrieval","score_opus":0.0076884039915145865,"score_gpt":0.2221833369569974,"score_spread":0.21449493296548283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146602332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963975,0.000018911398,0.000023312541,0.000004374256,3.4790187e-7,0.0000010960773,0.000042976375,0.0000043442033,0.00026495958],"genre_scores_gemma":[0.99953234,0.00001114008,0.00006036853,0.0000040215737,0.0000017898514,0.0000015626434,0.00025667332,0.0000026783762,0.00012939448],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983966,0.000018461087,0.0000067895253,0.000038864953,0.000036035126,0.000060145467],"domain_scores_gemma":[0.9993179,0.00007170478,0.0002793135,0.000043962034,0.00005576115,0.00023133987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001486636,0.0002573176,0.00025639994,0.0008492849,0.00051842234,0.0007367072,0.00034945176,0.00016950254,0.00094777165],"category_scores_gemma":[0.0005426883,0.00014711834,0.0002328344,0.00070075854,0.000338472,0.00025004748,0.0006640191,0.00017190626,0.0002696475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002685889,0.000067804045,0.9772372,0.00001144346,0.00005416858,0.0004451265,0.00041783694,0.0006900753,0.017553987,0.0003303451,0.00020310227,0.0027202994],"study_design_scores_gemma":[0.0000055458436,0.000040381885,0.99773765,0.0000012956024,0.000010831736,0.00017650651,0.00016926874,0.00097300066,0.0005802538,0.00005061589,0.0002506124,0.0000040555456],"about_ca_topic_score_codex":0.014443264,"about_ca_topic_score_gemma":0.016774522,"teacher_disagreement_score":0.014443264,"about_ca_system_score_codex":0.0006500101,"about_ca_system_score_gemma":0.00018868787,"threshold_uncertainty_score":0.028718412},"labels":[],"label_agreement":null},{"id":"W2146810479","doi":"10.1088/0004-637x/779/1/86","title":"A MEASUREMENT OF THE COSMIC MICROWAVE BACKGROUND DAMPING TAIL FROM THE 2500-SQUARE-DEGREE SPT-SZ SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":343,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"","keywords":"Cosmic microwave background; Physics; Astrophysics; Spectral index; CMB cold spot; South Pole Telescope; Cosmic background radiation; Spectral density; Redshift; Anisotropy; Multipole expansion; Cosmology; Astronomy; Spectral line; Galaxy; Optics","score_opus":0.03956137928336512,"score_gpt":0.24820165397896227,"score_spread":0.20864027469559715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146810479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9834562,0.000073568146,0.0031457222,0.0000567033,0.000009352106,0.000019120189,0.009655865,0.0001630457,0.0034204083],"genre_scores_gemma":[0.9774195,0.0001164405,0.0025206173,0.000025008227,0.000031783464,0.000031472424,0.01921853,0.0000373413,0.00059924636],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972886,0.000044162014,0.000012328923,0.000068136374,0.00011151311,0.000035003457],"domain_scores_gemma":[0.99862397,0.000130984,0.00046906996,0.00026211256,0.000221355,0.00029265851],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034093263,0.0004057886,0.00016955734,0.0014550462,0.00016813846,0.00037910978,0.00025245905,0.0001796201,0.0014306982],"category_scores_gemma":[0.0013342744,0.00016381813,0.00019174388,0.0016940944,0.00018990184,0.00031135083,0.0005331704,0.00030787132,0.00071976066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018588669,0.000046702837,0.9532752,0.00005290934,0.00015141566,0.00013672991,0.0002436628,0.0027450079,0.014702095,0.00078469585,0.0038122584,0.023863524],"study_design_scores_gemma":[0.000008831942,0.00004777231,0.9908799,0.0000034308132,0.000021329819,0.00013834285,0.000038458795,0.0023711373,0.0023591288,0.00014799462,0.0039758417,0.000007768878],"about_ca_topic_score_codex":0.0026433945,"about_ca_topic_score_gemma":0.004477942,"teacher_disagreement_score":0.0026433945,"about_ca_system_score_codex":0.0002172853,"about_ca_system_score_gemma":0.00015205231,"threshold_uncertainty_score":0.005256057},"labels":[],"label_agreement":null},{"id":"W2146844598","doi":"10.1086/421385","title":"Dust and Gas Obscuration in ELAIS Deep X‐Ray Survey Reddened Quasars","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Comisión Nacional de Investigación Científica y Tecnológica; National Astronomical Observatory of Japan; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Consejo Nacional de Investigaciones Científicas y Técnicas; National Science Foundation","keywords":"Quasar; Population; OVV quasar; Milky Way; Flux (metallurgy); Absorption (acoustics)","score_opus":0.01027384620862124,"score_gpt":0.21956196884989615,"score_spread":0.20928812264127492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146844598","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994634,0.000064428365,0.00001867324,0.0000058577352,4.3963107e-7,9.0534104e-7,0.00010500088,0.0000029127216,0.0003383132],"genre_scores_gemma":[0.9994698,0.00005112528,0.000032413325,0.000008021377,0.0000018357603,0.0000011139771,0.0002578122,0.000001924651,0.00017595505],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997962,0.00002522173,0.000022253345,0.00004675388,0.00005594682,0.000053664713],"domain_scores_gemma":[0.99881124,0.00018138504,0.00056459283,0.0001254143,0.00012779569,0.00018956055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035474717,0.000237018,0.00025931347,0.0014752855,0.00029702278,0.0008904188,0.00027432674,0.00018608554,0.0010475452],"category_scores_gemma":[0.0008756984,0.0001712094,0.00023335869,0.0005853499,0.00051125616,0.00033397184,0.0006043723,0.00019074058,0.0002058829],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045772376,0.000014319113,0.9949385,0.0000067173096,0.000025216339,0.00009262336,0.0002534686,0.000096153555,0.0032498313,0.000044470045,0.00003864756,0.0011942943],"study_design_scores_gemma":[6.4216636e-7,0.0000058758715,0.99962306,0.0000012334928,0.000003347201,0.00003704818,0.0000833635,0.000036998288,0.00013667994,0.000007579182,0.00006326091,8.2644107e-7],"about_ca_topic_score_codex":0.016380414,"about_ca_topic_score_gemma":0.01657903,"teacher_disagreement_score":0.016380414,"about_ca_system_score_codex":0.0003919962,"about_ca_system_score_gemma":0.00012485844,"threshold_uncertainty_score":0.032570183},"labels":[],"label_agreement":null},{"id":"W2146896318","doi":"10.1088/0004-637x/710/2/1247","title":"THE MASS DISTRIBUTION OF STARLESS AND PROTOSTELLAR CORES IN GOULD BELT CLOUDS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Astrophysics; Physics; James Clerk Maxwell Telescope; Molecular cloud; Serpens; Photometry (optics); Astronomy; Star formation; Young stellar object; Protostar; Galaxy; Stars","score_opus":0.006507419547790185,"score_gpt":0.23454592843440594,"score_spread":0.22803850888661575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146896318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99974746,0.000027603919,0.000016683298,0.0000054315337,1.7600416e-7,0.0000010409922,0.00006322584,0.0000038164294,0.00013472854],"genre_scores_gemma":[0.99972945,0.000012715053,0.000033833516,0.0000042422425,5.9003605e-7,8.143102e-7,0.00015666183,0.000001476891,0.00006022527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999068,0.000008741287,0.0000054368616,0.000021354432,0.000019382835,0.00003825133],"domain_scores_gemma":[0.9994894,0.00008169037,0.00016084831,0.00003126688,0.00005388781,0.00018294224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015502317,0.00013674592,0.00013695209,0.0018457957,0.00025644127,0.0004526536,0.00032115934,0.0002034134,0.0008911815],"category_scores_gemma":[0.00091196265,0.00008843809,0.00013081919,0.00061764993,0.00036705902,0.00029846595,0.00047209373,0.0000932268,0.00014104601],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000064591455,0.000010841774,0.99441975,0.000004025099,0.0000122850115,0.000057125846,0.00021160838,0.00012484538,0.0023864852,0.00013856325,0.00007900586,0.0024908783],"study_design_scores_gemma":[0.0000022115328,0.0000101960395,0.99923944,0.0000016097285,0.0000032491619,0.000042021842,0.00010496664,0.00036724462,0.000119868804,0.00004264669,0.000065035376,0.0000015708324],"about_ca_topic_score_codex":0.024894983,"about_ca_topic_score_gemma":0.04192023,"teacher_disagreement_score":0.024894983,"about_ca_system_score_codex":0.00066144805,"about_ca_system_score_gemma":0.00018271593,"threshold_uncertainty_score":0.049500167},"labels":[],"label_agreement":null},{"id":"W2146919530","doi":"10.1088/0004-637x/704/2/1433","title":"A 31 GHz SURVEY OF LOW-FREQUENCY SELECTED RADIO SOURCES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Spectral index; Sky; Cosmic microwave background; Radio telescope; Flux (metallurgy); Radio spectrum; Telescope; South Pole Telescope; Astronomy; Source counts; Population; Active galactic nucleus; Observatory; Microwave; COSMIC cancer database; Redshift; Spectral line; Galaxy; Optics","score_opus":0.00805004823391977,"score_gpt":0.21532840302273096,"score_spread":0.20727835478881118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2146919530","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98540395,0.00039333443,0.0018858396,0.00010506087,0.000009540897,0.000049448518,0.0053349556,0.00010215054,0.00671567],"genre_scores_gemma":[0.97399306,0.0004970157,0.0039541875,0.00013238486,0.000061133826,0.00006726633,0.017192267,0.000032113057,0.0040703854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969304,0.000044240693,0.0000149869065,0.00009576963,0.00008548396,0.000066458124],"domain_scores_gemma":[0.99922657,0.000063065876,0.00023202263,0.00010878779,0.00011632102,0.0002531173],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038476128,0.00021285,0.00020062753,0.0013313454,0.00032880926,0.00040256616,0.0002558154,0.00017082652,0.0030295367],"category_scores_gemma":[0.00052833935,0.0001631651,0.00020487772,0.0009898065,0.00011640761,0.0002450167,0.0006761785,0.00019939517,0.0017188126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000139304,0.000120282166,0.91978323,0.000065874505,0.00006537957,0.00035002822,0.0003041382,0.00086508854,0.023294082,0.0006265892,0.0075627333,0.046823245],"study_design_scores_gemma":[0.000007725545,0.000031825948,0.99428284,0.0000065683007,0.000009895561,0.00015695459,0.000030966225,0.0003557817,0.00049907516,0.00006227963,0.0045519494,0.0000042221336],"about_ca_topic_score_codex":0.005548991,"about_ca_topic_score_gemma":0.011466472,"teacher_disagreement_score":0.005548991,"about_ca_system_score_codex":0.00030514406,"about_ca_system_score_gemma":0.00040198426,"threshold_uncertainty_score":0.011033356},"labels":[],"label_agreement":null},{"id":"W2147008931","doi":"10.1086/508016","title":"High‐Energy Neutrino Astronomy Using Upward‐going Muons in Super‐Kamiokande I","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF","funders":"","keywords":"Physics; Super-Kamiokande; Neutrino; Muon; Flux (metallurgy); Astronomy; Neutrino detector; Neutrino astronomy; Astrophysics; Cosmic ray; Astroparticle physics; Nuclear physics; Particle physics; Neutrino oscillation; Solar neutrino","score_opus":0.0075143638441807,"score_gpt":0.20514571486581035,"score_spread":0.19763135102162965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147008931","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993599,0.00010530879,0.00012077697,0.0000060623097,9.170211e-7,0.0000033389656,0.00006453249,0.0000020407301,0.00033714963],"genre_scores_gemma":[0.9984798,0.00025670027,0.0005321353,0.000009848222,0.0000046451482,0.000007830369,0.00051629054,0.000003650789,0.00018919104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970835,0.000089474146,0.000018880835,0.00006353489,0.00006318853,0.000056652098],"domain_scores_gemma":[0.99860966,0.00047883863,0.00048469237,0.0001632037,0.00016614494,0.000097331336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048582474,0.00034311824,0.00033730778,0.0014833573,0.00041802844,0.0007153125,0.00030021454,0.00022202778,0.00042332447],"category_scores_gemma":[0.0011087671,0.0002386434,0.00057148584,0.001390928,0.00033641307,0.00033939414,0.00082649896,0.00027561764,0.000114004586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068944035,0.00006462837,0.95829713,0.00007528727,0.00033391343,0.0010641917,0.00087705057,0.0008899498,0.025416212,0.00024226689,0.00010964299,0.011940287],"study_design_scores_gemma":[0.000019175342,0.00023135249,0.9868519,0.000019129899,0.00016697307,0.00077311427,0.00043796873,0.0005917723,0.009491112,0.00014554459,0.0012526463,0.000019306799],"about_ca_topic_score_codex":0.0060371263,"about_ca_topic_score_gemma":0.010556474,"teacher_disagreement_score":0.0060371263,"about_ca_system_score_codex":0.0002609357,"about_ca_system_score_gemma":0.00019107827,"threshold_uncertainty_score":0.012003958},"labels":[],"label_agreement":null},{"id":"W2147063522","doi":"10.1088/0004-637x/763/2/141","title":"MOA-2010-BLG-523: “FAILED PLANET” = RS CVn STAR","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Japan Society for the Promotion of Science; National Research Foundation of Korea; Fonds National de la Recherche Luxembourg; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Qatar National Research Fund; Korea Research Council of Fundamental Science and Technology; Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Vetenskapsrådet; National Science Foundation","keywords":"Gravitational microlensing; Physics; Light curve; Bulge; Astrophysics; Planet; Astronomy; Planetary system; Stars; Star (game theory); Variable star","score_opus":0.009344945196321269,"score_gpt":0.2031899172083339,"score_spread":0.19384497201201265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147063522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99658656,0.000109700224,0.0002623618,0.000059582148,0.000016158978,0.0000049395308,0.0005843722,0.00007212363,0.0023042106],"genre_scores_gemma":[0.99883205,0.000012964009,0.00020196903,0.000020680542,0.0000053151953,0.0000014217208,0.0005266595,0.000015002902,0.0003839386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989736,0.0000063063408,0.0000056859058,0.00004452527,0.000020508252,0.000025572244],"domain_scores_gemma":[0.9996805,0.00002647793,0.00010489536,0.00005681153,0.000044200286,0.00008714353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012875765,0.0002093804,0.00020465869,0.00055351574,0.00068988366,0.00047684624,0.00025865395,0.00039098237,0.0015821191],"category_scores_gemma":[0.00032812252,0.00008372583,0.00013148865,0.00046688522,0.00049328397,0.00025985946,0.00040438125,0.0003509829,0.00048843434],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000717378,0.0001095865,0.8363629,0.00011701077,0.00013010047,0.004615811,0.0006639052,0.0003333842,0.13152994,0.00075167377,0.0023444823,0.02232378],"study_design_scores_gemma":[0.000007120367,0.00011514641,0.9782906,0.0000067887445,0.0000221856,0.005702955,0.00023329437,0.0003967873,0.010264825,0.00010103115,0.004845786,0.000013619579],"about_ca_topic_score_codex":0.0072593,"about_ca_topic_score_gemma":0.013594748,"teacher_disagreement_score":0.0072593,"about_ca_system_score_codex":0.00052941643,"about_ca_system_score_gemma":0.00013493717,"threshold_uncertainty_score":0.014434099},"labels":[],"label_agreement":null},{"id":"W2147284265","doi":"10.1086/379539","title":"Estimates of Cosmological Parameters Using the Cosmic Microwave Background Angular Power Spectrum of ACBAR","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Astrophysics; Cosmic background radiation; Cosmology; Inflation (cosmology); Spectral density; Bolometer; Sunyaev–Zel'dovich effect; Hubble's law; Cold dark matter; COSMIC cancer database; Dark energy; Amplitude; Anisotropy; Astronomy; Detector; Statistics","score_opus":0.01801881215433187,"score_gpt":0.264447942142565,"score_spread":0.24642912998823313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147284265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.923197,0.00042979236,0.06727503,0.000070492264,0.000013989937,0.000021620644,0.0011597009,0.00049086683,0.007341435],"genre_scores_gemma":[0.97731596,0.00018080637,0.021013089,0.000015331167,0.000019567839,0.00001446097,0.0011859657,0.00004765283,0.000207139],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966717,0.000099762314,0.000011720133,0.00007234057,0.00012385842,0.000025238925],"domain_scores_gemma":[0.9981104,0.00046651126,0.0006319245,0.00043669104,0.00023964526,0.00011478366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087429903,0.00062589196,0.0002451457,0.0024472473,0.00028258475,0.0006493429,0.0003596955,0.00020316374,0.0010730835],"category_scores_gemma":[0.0037126986,0.00021536094,0.00026120627,0.0015284736,0.00028917412,0.00070023513,0.00050831056,0.00044722826,0.00036550465],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021378984,0.00013530444,0.80221534,0.00012274939,0.0003835778,0.00022421569,0.0003293652,0.037822943,0.039095834,0.015122752,0.0011335538,0.1032006],"study_design_scores_gemma":[0.000049837552,0.00017607551,0.8068479,0.000058365273,0.00013195624,0.0006289183,0.00014215932,0.1292594,0.03353518,0.01999286,0.009074159,0.00010319739],"about_ca_topic_score_codex":0.0021591051,"about_ca_topic_score_gemma":0.003316542,"teacher_disagreement_score":0.0024472473,"about_ca_system_score_codex":0.0003106339,"about_ca_system_score_gemma":0.00012198846,"threshold_uncertainty_score":0.0046237707},"labels":[],"label_agreement":null},{"id":"W2147297461","doi":"10.1088/0004-637x/751/2/90","title":"PANCHROMATIC OBSERVATIONS OF THE TEXTBOOK GRB 110205A: CONSTRAINING PHYSICAL MECHANISMS OF PROMPT EMISSION AND AFTERGLOW","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministerio de Ciencia e Innovación; Goddard Space Flight Center; National Science Foundation; Junta de Andalucía; National Aeronautics and Space Administration","keywords":"Physics; Afterglow; Astrophysics; Gamma-ray burst; Light curve; Redshift; Synchrotron; Spectral line; Emission spectrum; Spectral energy distribution; Shock (circulatory); Extrapolation; Astronomy; Optics; Galaxy","score_opus":0.01789280347968868,"score_gpt":0.23229961781144765,"score_spread":0.21440681433175895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147297461","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951443,0.00025516073,0.00040469534,0.000041054944,0.000008206541,0.00001080349,0.0021179598,0.00007664413,0.0019411144],"genre_scores_gemma":[0.99323565,0.00018773811,0.0013641035,0.000044107015,0.000027390823,0.000013888819,0.0044940338,0.000018304207,0.000614855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999418,0.0000032229475,0.000003050963,0.000019935458,0.000015066828,0.000016930046],"domain_scores_gemma":[0.9998054,0.000016821521,0.00007079741,0.000023012082,0.00001676854,0.00006719593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000091527596,0.00032886036,0.00025869734,0.00095489906,0.0002641079,0.00034135868,0.00025757946,0.0002190712,0.0009783375],"category_scores_gemma":[0.0001224516,0.00019284029,0.00027248435,0.00085626444,0.00016485232,0.00018903342,0.0004246267,0.0002890319,0.0003965527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011141576,0.00037159168,0.67683315,0.00026609344,0.00021164319,0.0027881619,0.00041431838,0.0021807158,0.2648828,0.00044365684,0.0036591394,0.04683457],"study_design_scores_gemma":[0.00001011173,0.00009607183,0.9936872,0.000005627156,0.000033792636,0.0007753022,0.00006979949,0.0008588838,0.002604019,0.00006825493,0.0017808743,0.000010075373],"about_ca_topic_score_codex":0.0040039904,"about_ca_topic_score_gemma":0.010915735,"teacher_disagreement_score":0.0040039904,"about_ca_system_score_codex":0.00019445256,"about_ca_system_score_gemma":0.00015289878,"threshold_uncertainty_score":0.007961392},"labels":[],"label_agreement":null},{"id":"W2147319497","doi":"10.1086/520625","title":"Is There Evidence for a Hubble Bubble? The Nature of Type Ia Supernova Colors and Dust in External Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":166,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Supernova; Milky Way; Galaxy; Light curve; Redshift; Hubble's law; Luminosity; Cosmology; Astronomy","score_opus":0.02225342682937372,"score_gpt":0.29489030685914813,"score_spread":0.27263688002977443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147319497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99493104,0.00095457176,0.00021566986,0.00047755337,0.000018255452,0.0000072523335,0.00055581925,0.000017164086,0.0028225658],"genre_scores_gemma":[0.99871576,0.00027962722,0.00008809995,0.00012895677,0.00004826618,0.0000022720485,0.00029856517,0.000006947331,0.00043161263],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998648,0.000024950245,0.000013471165,0.000029031859,0.000027840115,0.000039807383],"domain_scores_gemma":[0.9943176,0.0022620386,0.0015444921,0.0004114649,0.00040514677,0.001059283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062026444,0.00015737998,0.00024411827,0.0012842048,0.00021707988,0.00076383946,0.000478122,0.0006641627,0.010662425],"category_scores_gemma":[0.0028556078,0.00014168683,0.00017278215,0.0008725027,0.000946282,0.0007679163,0.0002999905,0.00038383278,0.00068211276],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023512311,0.000045651646,0.9916123,0.000034903063,0.000033788005,0.00017053318,0.00013778782,0.000033216173,0.0023529504,0.0003034388,0.00044561116,0.0045945416],"study_design_scores_gemma":[0.000016998856,0.000058516973,0.9977331,0.00002640952,0.000033977376,0.00043098404,0.0003600608,0.00014107468,0.00034107757,0.00039889035,0.0004526896,0.0000063049574],"about_ca_topic_score_codex":0.0084616225,"about_ca_topic_score_gemma":0.011100416,"teacher_disagreement_score":0.010662425,"about_ca_system_score_codex":0.00026603186,"about_ca_system_score_gemma":0.00019998295,"threshold_uncertainty_score":0.035669386},"labels":[],"label_agreement":null},{"id":"W2147441532","doi":"10.1086/424956","title":"A Genetic Algorithm–based Exploration of Three Filament Models: A Case for the Magnetic Support of the G11.11−0.12 Infrared‐dark Cloud","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Magnetic field; Polarization (electrochemistry); Protein filament; Molecular cloud; Magnetic cloud; Magnetic structure; Dynamo; Plane (geometry)","score_opus":0.026459755309105007,"score_gpt":0.2392093861736215,"score_spread":0.21274963086451648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147441532","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97460055,0.00008829772,0.021719497,0.000267466,0.000005452638,0.000042075317,0.00006334652,0.000045475703,0.003167834],"genre_scores_gemma":[0.9731889,0.00006728338,0.025921745,0.00005655523,0.000008075364,0.000063135914,0.0001134135,0.0000109958055,0.0005698393],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999157,0.000040949973,0.000002950364,0.00001407889,0.000009219383,0.000017083257],"domain_scores_gemma":[0.9991478,0.0006474396,0.00006715192,0.000032121578,0.00005554638,0.000049931346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005588378,0.0004196297,0.00037103845,0.00071408995,0.0005656578,0.0006997482,0.0006855639,0.00082739495,0.0007152171],"category_scores_gemma":[0.002021629,0.00027509913,0.0005481126,0.0003148171,0.0004928415,0.00035191636,0.00038219386,0.0003977578,0.0000417995],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009000832,0.00008134739,0.0077339737,0.00001886078,0.00003748589,0.00016325375,0.000081531616,0.9784626,0.00085247715,0.005646259,0.00022214539,0.006610141],"study_design_scores_gemma":[0.000017907098,0.000025610963,0.0005559062,0.0000031415245,0.0000093351255,0.000009766255,0.000028497485,0.99790776,0.000092466056,0.0012546551,0.000092019094,0.0000030651565],"about_ca_topic_score_codex":0.009098832,"about_ca_topic_score_gemma":0.009827763,"teacher_disagreement_score":0.009098832,"about_ca_system_score_codex":0.00072187674,"about_ca_system_score_gemma":0.00066894654,"threshold_uncertainty_score":0.018091738},"labels":[],"label_agreement":null},{"id":"W2147445613","doi":"10.1086/377528","title":"Evolution of Cluster Elliptical Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Luminosity function; Fundamental plane (elliptical galaxies); Elliptical galaxy; Astronomy; Galaxy; Redshift; Surface brightness fluctuation; Galaxy cluster; Luminosity; Luminous infrared galaxy; Galaxy groups and clusters; Brightest cluster galaxy; Population; Stellar population; Lenticular galaxy; Star formation","score_opus":0.0064727229654568804,"score_gpt":0.2061627789308473,"score_spread":0.19969005596539044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147445613","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924664,0.00026049188,0.00016182919,0.00017031307,0.0000039670567,0.0000038787275,0.0010612254,0.000068449575,0.005803274],"genre_scores_gemma":[0.99740005,0.000039132156,0.000083883744,0.000010895299,0.0000029056162,0.0000012749603,0.00049612246,0.000012310883,0.001953545],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983096,0.000021421383,0.000004300819,0.000066854074,0.000024935482,0.000051585157],"domain_scores_gemma":[0.99880826,0.00017612037,0.0002814221,0.0001452678,0.0002227005,0.00036616815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030956307,0.00009854174,0.00014584254,0.0012256129,0.00034331816,0.0011145931,0.00023896352,0.0003301307,0.008809735],"category_scores_gemma":[0.0015760859,0.00012545433,0.00015708536,0.0005871475,0.00032839793,0.00035403518,0.00046109987,0.0001855763,0.0021753854],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000100583035,0.00002045529,0.9727233,0.000013899605,0.00005627875,0.00009304282,0.0005338928,0.0019981228,0.003676549,0.0030792705,0.0035427215,0.014161895],"study_design_scores_gemma":[0.0000010802365,0.0000068448285,0.99812144,0.0000025795518,0.0000042040265,0.000042920346,0.00010786646,0.0006570428,0.00009568658,0.00017965806,0.0007778801,0.0000026372106],"about_ca_topic_score_codex":0.02498176,"about_ca_topic_score_gemma":0.027107455,"teacher_disagreement_score":0.02498176,"about_ca_system_score_codex":0.001100103,"about_ca_system_score_gemma":0.00024030745,"threshold_uncertainty_score":0.049672723},"labels":[],"label_agreement":null},{"id":"W2147638840","doi":"10.1086/429083","title":"The Impact of Small‐Scale Structure on Cosmological Ionization Fronts and Reionization","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; University of California, Santa Barbara; National Science Foundation","keywords":"Reionization; Physics; Astrophysics; Cosmic microwave background; Intergalactic travel; Ionization; Redshift; Quasar; Photon; Optical depth; Astronomy; Galaxy; Optics; Quantum mechanics; Anisotropy","score_opus":0.006099933555234623,"score_gpt":0.21587206074836887,"score_spread":0.20977212719313426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147638840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99304295,0.0003795061,0.0010273866,0.00016059325,0.000008043727,0.0000079004785,0.00013049367,0.000038530692,0.005204594],"genre_scores_gemma":[0.9987565,0.00016580528,0.0001708756,0.000019306826,0.0000067858705,0.0000017377486,0.00007049581,0.00001695325,0.0007914666],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986565,0.000021804095,0.0000038110682,0.000022991224,0.000028053273,0.000057664325],"domain_scores_gemma":[0.99843866,0.0005344238,0.00044601326,0.00013756563,0.000105815765,0.00033751412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027302394,0.0003797026,0.00020821318,0.0006056957,0.00039797914,0.00082583376,0.000387652,0.0004600131,0.0031762165],"category_scores_gemma":[0.0022498297,0.00025393162,0.00045063056,0.0003560922,0.0005847332,0.0007788289,0.00094639097,0.00065744057,0.00033155637],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007596513,0.00038611417,0.4504369,0.000339342,0.00046436553,0.0026764038,0.0013652373,0.33636317,0.12797813,0.024629178,0.0026197287,0.051981755],"study_design_scores_gemma":[0.00004644445,0.00021610406,0.7821766,0.00003877109,0.00011580585,0.00037727918,0.00044409835,0.1941746,0.014238925,0.006029232,0.0020648101,0.000077354314],"about_ca_topic_score_codex":0.009031761,"about_ca_topic_score_gemma":0.0045796884,"teacher_disagreement_score":0.009031761,"about_ca_system_score_codex":0.0008159322,"about_ca_system_score_gemma":0.000305869,"threshold_uncertainty_score":0.017958403},"labels":[],"label_agreement":null},{"id":"W2147710137","doi":"10.1086/502677","title":"Nanodiamond as a Possible Carrier of Extended Red Emission","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Diamond and Carbon-based Materials Research","field":"Materials Science","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Nanodiamond; Photoluminescence; Physics; Luminescence; Excitation; Diamond; Wavelength; Annealing (glass); Optoelectronics; Irradiation; Optics; Materials science","score_opus":0.007710720355299098,"score_gpt":0.2538017392925332,"score_spread":0.2460910189372341,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147710137","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98864883,0.0011810551,0.0063250405,0.00010279457,0.00002750053,0.000016116866,0.000094111245,0.00010106836,0.0035034965],"genre_scores_gemma":[0.9916129,0.00036332497,0.005157794,0.0000253882,0.0000030308033,0.000009013126,0.00009931478,0.000012731653,0.002716458],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999628,0.000004535615,0.000001741446,0.000013953035,0.000010618829,0.000006341717],"domain_scores_gemma":[0.99991727,0.000032110373,0.0000141747805,0.000010823281,0.000016008256,0.000009601075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009540273,0.00012056568,0.000096186755,0.00015199925,0.00018054887,0.00035137645,0.00023350425,0.0002900795,0.0006220734],"category_scores_gemma":[0.0001764392,0.00009363752,0.00009345483,0.000080062804,0.00016348247,0.00027579427,0.00013539317,0.0001958817,0.0001497437],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000066843684,0.000016544138,0.00035154176,0.000071533635,0.000003890602,0.00011410687,0.000028515618,0.00030066966,0.9929287,0.002335476,0.000089606394,0.0036925892],"study_design_scores_gemma":[0.000009235122,0.00006723703,0.00066513644,0.0000071249374,0.000008237735,0.00018853045,0.000015756868,0.0033286603,0.99179614,0.00040690956,0.0035018572,0.000005100016],"about_ca_topic_score_codex":0.00053623295,"about_ca_topic_score_gemma":0.0007770316,"teacher_disagreement_score":0.0006220734,"about_ca_system_score_codex":0.00047866214,"about_ca_system_score_gemma":0.0001546023,"threshold_uncertainty_score":0.0034729242},"labels":[],"label_agreement":null},{"id":"W2147778163","doi":"10.1088/0004-637x/792/2/97","title":"FUNDAMENTAL LIMITATIONS OF HIGH CONTRAST IMAGING SET BY SMALL SAMPLE STATISTICS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":371,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Contrast (vision); Sample size determination; Statistics; Statistical power; False alarm; Robustness (evolution); CLs upper limits; Gaussian; Confidence interval; Statistical hypothesis testing; Mathematics; Algorithm; Computer science; Physics; Artificial intelligence","score_opus":0.020066449198463267,"score_gpt":0.2257437173503544,"score_spread":0.20567726815189113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147778163","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01798072,0.007061304,0.9647593,0.0031482677,0.00031025827,0.00009020252,0.00032884494,0.0006106928,0.0057104593],"genre_scores_gemma":[0.67539877,0.0075994204,0.3065953,0.004046416,0.0017015481,0.0006224494,0.00079904456,0.00087715045,0.0023599518],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.97863436,0.00980625,0.0012806501,0.0034014282,0.0063099684,0.00056743046],"domain_scores_gemma":[0.6598396,0.31006104,0.009804641,0.0127229355,0.006825018,0.0007468334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.032670103,0.0011276794,0.0025279736,0.0015178907,0.0011784997,0.0048484015,0.0040556993,0.002477945,0.0021674559],"category_scores_gemma":[0.21857296,0.0010194032,0.0010372334,0.0013356883,0.007311999,0.007391383,0.0044408557,0.0050955666,0.0007250538],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085978664,0.00011875395,0.023227029,0.0029095165,0.00082801806,0.0018904404,0.0014080873,0.12173049,0.01643671,0.6151763,0.009748826,0.205666],"study_design_scores_gemma":[0.000077335106,0.00023223367,0.006864628,0.00062059285,0.00017275366,0.0020309817,0.00022213424,0.21340585,0.019879034,0.743441,0.012839585,0.00021396553],"about_ca_topic_score_codex":0.0019810672,"about_ca_topic_score_gemma":0.00095714343,"teacher_disagreement_score":0.032670103,"about_ca_system_score_codex":0.00199604,"about_ca_system_score_gemma":0.0011601637,"threshold_uncertainty_score":0.17277807},"labels":[],"label_agreement":null},{"id":"W2147904130","doi":"10.1086/381424","title":"M31’s Undisturbed Thin Disk of Globular Clusters","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Globular cluster; Astrophysics; Thick disk; Physics; Thin disk; Milky Way; Astronomy; Galaxy; Star cluster; Halo","score_opus":0.008023231211211942,"score_gpt":0.21917505803361334,"score_spread":0.2111518268224014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147904130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911788,0.00034077012,0.0006803334,0.00011457482,0.000008910573,0.0000061102924,0.00017976122,0.000036062404,0.007454723],"genre_scores_gemma":[0.9971943,0.00013285622,0.0008487114,0.000061705796,0.000007848784,0.0000048584507,0.00036368548,0.000008016314,0.0013779736],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999151,0.000004928155,0.0000027287379,0.000023239927,0.0000225435,0.000031453816],"domain_scores_gemma":[0.9997539,0.000025913429,0.00005074484,0.0000601145,0.000037150367,0.000072081486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108130895,0.0001907144,0.00013043865,0.00041944152,0.0011575796,0.00065535086,0.00040535672,0.0003189204,0.0021986386],"category_scores_gemma":[0.00059100887,0.00013048307,0.0001427032,0.00057769846,0.00042535088,0.00070691836,0.0008104684,0.0002478496,0.00075631356],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008777904,0.0001574853,0.647369,0.00019839624,0.000076578195,0.005236242,0.0023846803,0.0076788263,0.23555842,0.033256464,0.010096665,0.057109382],"study_design_scores_gemma":[0.00002960464,0.00021930055,0.909107,0.00004807146,0.00003497133,0.006135082,0.00091551355,0.017714696,0.020038035,0.00928709,0.03642307,0.00004745965],"about_ca_topic_score_codex":0.00678359,"about_ca_topic_score_gemma":0.0052963425,"teacher_disagreement_score":0.00678359,"about_ca_system_score_codex":0.00062864204,"about_ca_system_score_gemma":0.00034350838,"threshold_uncertainty_score":0.013488233},"labels":[],"label_agreement":null},{"id":"W2147913035","doi":"10.1088/0004-637x/776/1/20","title":"PSR J1723–2837: AN ECLIPSING BINARY RADIO MILLISECOND PULSAR","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Pulsar; Millisecond pulsar; Astrophysics; Orbital period; Binary pulsar; Astronomy; Roche lobe; Pulsar planet; Photometry (optics); Binary star; Stars","score_opus":0.013417753812217338,"score_gpt":0.3025394643073052,"score_spread":0.2891217104950879,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147913035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992434,0.00005779862,0.0000465435,0.000016703169,0.0000032637088,0.000004814313,0.00007142195,0.000006049568,0.0005501449],"genre_scores_gemma":[0.99850947,0.00009813193,0.0002594277,0.0000325468,0.00001776307,0.00000795431,0.00065098563,0.000006810043,0.00041687462],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990237,0.000008599837,0.000007213549,0.000025203633,0.000031677566,0.000024809431],"domain_scores_gemma":[0.9997875,0.000019896432,0.00006278984,0.000017591676,0.000030952833,0.000081238264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013465233,0.0002197333,0.0003067185,0.00060018164,0.0007043395,0.00053726614,0.00035086198,0.00026379383,0.0008865108],"category_scores_gemma":[0.00028837676,0.00006657702,0.00012392744,0.00070842303,0.00027779408,0.00024442872,0.00037875757,0.00021963964,0.0005652194],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005107144,0.0006000161,0.8442577,0.0001187265,0.00012195071,0.015245351,0.0011803395,0.0010719076,0.10486949,0.0008159054,0.0023555267,0.028852332],"study_design_scores_gemma":[0.000049704035,0.0007922948,0.9737159,0.000010490466,0.00004364763,0.008048366,0.001130632,0.0021040575,0.0065597724,0.00027882037,0.0072482205,0.000018163173],"about_ca_topic_score_codex":0.003523072,"about_ca_topic_score_gemma":0.0051576993,"teacher_disagreement_score":0.003523072,"about_ca_system_score_codex":0.00031983902,"about_ca_system_score_gemma":0.00028066925,"threshold_uncertainty_score":0.007005155},"labels":[],"label_agreement":null},{"id":"W2147922111","doi":"10.1086/368019","title":"Interstellar Deuterium, Nitrogen, and Oxygen Abundances toward GD 246, WD 2331−475, HZ 21, and Lanning 23: Results from the<i>FUSE</i>Mission","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Line-of-sight; Local Bubble; Astrophysics; Spectral line; Line (geometry); Interstellar medium; Astronomy; Galaxy","score_opus":0.0175108664601518,"score_gpt":0.24154071746804215,"score_spread":0.22402985100789036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2147922111","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960432,0.00009059229,0.00015192752,0.000022585176,0.0000035440755,0.000006587628,0.0015374926,0.000044297587,0.0020997522],"genre_scores_gemma":[0.9965061,0.00006892971,0.0003147712,0.000032262826,0.0000049361934,0.0000058108462,0.0022295727,0.000017232278,0.00082032394],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999082,0.0000036884164,0.000003406569,0.000039233437,0.000023424049,0.000021931679],"domain_scores_gemma":[0.9998542,0.000012916306,0.000040608888,0.00001172493,0.00002282001,0.00005766614],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021555054,0.00048152122,0.00037624422,0.00073291705,0.0007037699,0.0004530749,0.00038462668,0.00041712564,0.0010308566],"category_scores_gemma":[0.00017540774,0.00024291975,0.00034345072,0.0004783634,0.0002707196,0.00036582132,0.00057456404,0.00027347333,0.0004511592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0041764714,0.0003185236,0.6448287,0.00015118807,0.0004331782,0.00088026095,0.0011803984,0.00634859,0.3157254,0.00078284007,0.0027479199,0.02242657],"study_design_scores_gemma":[0.00010603244,0.00019320968,0.9685647,0.0000100059315,0.0001813369,0.00031331342,0.00028443948,0.0025474874,0.025281634,0.0001518028,0.0023387305,0.000027415244],"about_ca_topic_score_codex":0.028250393,"about_ca_topic_score_gemma":0.049662437,"teacher_disagreement_score":0.028250393,"about_ca_system_score_codex":0.0006516159,"about_ca_system_score_gemma":0.0002624349,"threshold_uncertainty_score":0.056171894},"labels":[],"label_agreement":null},{"id":"W2148161570","doi":"10.1088/0004-637x/734/1/44","title":"<i>CHANDRA</i>OBSERVATIONS OF THE HIGH-MAGNETIC-FIELD RADIO PULSAR J1718–3718","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Astrophysics; Magnetar; Neutron star; Luminosity; X-ray pulsar; Astronomy; Black-body radiation; Magnetic field; Millisecond pulsar; Radiation; Galaxy; Nuclear physics","score_opus":0.02246792380779335,"score_gpt":0.27113303417215406,"score_spread":0.2486651103643607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148161570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96614957,0.0020760822,0.0014326223,0.0004440508,0.00012875917,0.000073992014,0.008302131,0.0007013609,0.020691516],"genre_scores_gemma":[0.9762393,0.001632172,0.0069058896,0.00035412872,0.00029603238,0.00004590856,0.011101649,0.00016560144,0.0032592227],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987555,0.0000093397175,0.00001091248,0.00002703501,0.000042264128,0.00003472821],"domain_scores_gemma":[0.998976,0.00008376243,0.00040183795,0.00015531057,0.00019697347,0.00018618864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022976333,0.0003501374,0.00025088043,0.0019238209,0.00043254532,0.00075105974,0.0003194837,0.0001586332,0.0048787454],"category_scores_gemma":[0.00061083474,0.00014560563,0.00013584475,0.0012859881,0.00032704134,0.00042752447,0.00062209915,0.00031264205,0.0012261904],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038877924,0.00016280606,0.7252462,0.0004227534,0.00021609908,0.001193584,0.00044103683,0.00038071544,0.12285521,0.0008413221,0.021079704,0.1267718],"study_design_scores_gemma":[0.000031677766,0.000066373264,0.9606038,0.00003319687,0.000056155353,0.001595945,0.00012719221,0.00018734737,0.007865329,0.00022075759,0.029196938,0.0000153813],"about_ca_topic_score_codex":0.003885591,"about_ca_topic_score_gemma":0.009614722,"teacher_disagreement_score":0.0048787454,"about_ca_system_score_codex":0.00026866441,"about_ca_system_score_gemma":0.00032357065,"threshold_uncertainty_score":0.016321063},"labels":[],"label_agreement":null},{"id":"W2148205276","doi":"10.1088/0004-637x/732/1/54","title":"PREDICTING THE DETECTABILITY OF OSCILLATIONS IN SOLAR-TYPE STARS OBSERVED BY<i>KEPLER</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency","funders":"Science and Technology Facilities Council","keywords":"Asteroseismology; Physics; Kepler; Exoplanet; Stars; Astronomy; Astrophysics; RADIUS; Planet; Magnitude (astronomy)","score_opus":0.032005639954632445,"score_gpt":0.2228319467508424,"score_spread":0.19082630679620993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148205276","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95057625,0.00094377116,0.040967137,0.00037961372,0.000026270824,0.000029287914,0.00086372707,0.00027191857,0.0059420187],"genre_scores_gemma":[0.98835284,0.00029884116,0.010404824,0.000033735894,0.000028080047,0.00000928834,0.00067523966,0.00002946996,0.00016764252],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997247,0.00006791371,0.000045098946,0.000084551495,0.00005018624,0.000027616536],"domain_scores_gemma":[0.9963666,0.0020569442,0.00078782433,0.0003054393,0.00029257423,0.0001905657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001136439,0.00041020964,0.0002748946,0.0012429536,0.00034021764,0.0012727263,0.00041272317,0.0006851338,0.00051767786],"category_scores_gemma":[0.0070412927,0.000320738,0.00030392405,0.00062956684,0.00053456216,0.0015048577,0.00077438157,0.00062975136,0.00040050893],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000106461724,0.00002447212,0.9492756,0.000055570075,0.000073672745,0.000085993954,0.0001486955,0.0070812497,0.014881156,0.0017449817,0.00035179796,0.026170347],"study_design_scores_gemma":[0.0000140159,0.000121706595,0.950073,0.000034490506,0.000067710214,0.00043247628,0.00038791925,0.025434393,0.014613933,0.0065546427,0.0022058624,0.000059847927],"about_ca_topic_score_codex":0.0011407884,"about_ca_topic_score_gemma":0.0018265323,"teacher_disagreement_score":0.0012727263,"about_ca_system_score_codex":0.00018873248,"about_ca_system_score_gemma":0.00012460322,"threshold_uncertainty_score":0.006010115},"labels":[],"label_agreement":null},{"id":"W2148257426","doi":"10.1086/523839","title":"Confidence Level and Sensitivity Limits in High‐Contrast Imaging","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Speckle pattern; Point spread function; Sensitivity (control systems); Adaptive optics; Noise (video); Speckle noise; Pixel; Telescope; Intensity (physics); Speckle imaging","score_opus":0.02219459991229598,"score_gpt":0.23200367800397478,"score_spread":0.2098090780916788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148257426","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.35351267,0.00093114213,0.6370635,0.00061301934,0.000036134406,0.00004134924,0.00010647864,0.00043680498,0.007258904],"genre_scores_gemma":[0.97109365,0.00013569005,0.028255152,0.00007007115,0.000021069878,0.00003127202,0.0000841738,0.000035763187,0.00027305938],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99515235,0.0017076692,0.00022087997,0.00061663194,0.0019410421,0.0003614396],"domain_scores_gemma":[0.89617276,0.09058093,0.0047117197,0.0042861803,0.0034809895,0.0007673924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.009421757,0.00034506564,0.00046910037,0.0012729125,0.00053267746,0.0022488453,0.0015559508,0.0015816981,0.0007570808],"category_scores_gemma":[0.08815761,0.00054267823,0.0006196272,0.0007325637,0.0030621544,0.0020239796,0.0018401159,0.0011371153,0.00021327539],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006241738,0.0001267381,0.033113986,0.00034461735,0.0001971107,0.00090753625,0.0005735932,0.6961918,0.02649119,0.18498713,0.00090915104,0.055532906],"study_design_scores_gemma":[0.000021927628,0.00012624617,0.010504298,0.00006887228,0.000024286213,0.00058212475,0.00007296819,0.91322976,0.016613638,0.05803428,0.00064704556,0.00007457722],"about_ca_topic_score_codex":0.0020444598,"about_ca_topic_score_gemma":0.0006107786,"teacher_disagreement_score":0.009421757,"about_ca_system_score_codex":0.0014132815,"about_ca_system_score_gemma":0.0007483463,"threshold_uncertainty_score":0.049827576},"labels":[],"label_agreement":null},{"id":"W2148439125","doi":"10.1086/374406","title":"Halting Planet Migration by Photoevaporation from the Central Source","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; National Research Council Canada; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Photoevaporation; Planet; Physics; Planetary migration; Gas giant; Astrophysics; Astronomy; Jupiter (rocket family); Kepler-47; Stars; Astrobiology; Planetary system; Exoplanet; Protoplanetary disk","score_opus":0.007205989467708165,"score_gpt":0.20405933391198666,"score_spread":0.1968533444442785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148439125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964515,0.00031209222,0.0013324904,0.000070091126,0.000007804601,0.00000486811,0.000017031085,0.000118504075,0.0016855609],"genre_scores_gemma":[0.99864405,0.0001448704,0.000602834,0.000023447841,0.000005003377,0.0000052774476,0.00003532754,0.000014440796,0.00052466255],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999479,0.0000048686056,0.000002574899,0.000010221657,0.000010927464,0.000023355225],"domain_scores_gemma":[0.9996742,0.000083174935,0.00008213062,0.00008562423,0.000031724023,0.000043253676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110049055,0.0001596686,0.0002480912,0.00013286051,0.00025061434,0.0003555823,0.00029328614,0.0003027294,0.0010889216],"category_scores_gemma":[0.0005201128,0.00013774024,0.00015218866,0.00011314911,0.00028541285,0.00043374745,0.0005577341,0.00033784253,0.00043381195],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053971354,0.00006479945,0.036759026,0.00019424483,0.00005105704,0.001201144,0.00036493974,0.004600988,0.91466993,0.0018373603,0.0008020245,0.038914796],"study_design_scores_gemma":[0.00015791545,0.00072348,0.1141764,0.000042114858,0.00010191209,0.007891432,0.0006636079,0.026120396,0.8257999,0.0059064208,0.01837042,0.00004607863],"about_ca_topic_score_codex":0.00049223466,"about_ca_topic_score_gemma":0.00040026812,"teacher_disagreement_score":0.0010889216,"about_ca_system_score_codex":0.00014339462,"about_ca_system_score_gemma":0.00015513066,"threshold_uncertainty_score":0.0036427975},"labels":[],"label_agreement":null},{"id":"W2148452795","doi":"10.1088/0004-637x/719/2/1553","title":"<i>AKARI</i>AND BLAST OBSERVATIONS OF THE CASSIOPEIA A SUPERNOVA REMNANT AND SURROUNDING INTERSTELLAR MEDIUM","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Office of Polar Programs; Japan Aerospace Exploration Agency; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Korea Science and Engineering Foundation; National Aeronautics and Space Administration; Canadian Space Agency; National Science Foundation","keywords":"Physics; Astrophysics; Extinction (optical mineralogy); Supernova remnant; Interstellar medium; Cassiopeia A; Cosmic dust; Population; Ejecta; Molecular cloud; Astronomy; Supernova; Galaxy","score_opus":0.013349596853833122,"score_gpt":0.21845130620098754,"score_spread":0.2051017093471544,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148452795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98826885,0.0002865842,0.0014599899,0.00008733517,0.000030711486,0.00002107897,0.0053074723,0.00032595656,0.0042120246],"genre_scores_gemma":[0.9839447,0.0002499436,0.0061494457,0.000058073325,0.00005500868,0.000023028639,0.008567471,0.00005847987,0.0008938],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993527,0.000004137637,0.0000048085576,0.000018963123,0.0000238009,0.000012968356],"domain_scores_gemma":[0.99970466,0.000028266939,0.00010037569,0.00005820662,0.000045661116,0.00006290984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018516483,0.00023852556,0.00016719027,0.0015471876,0.0002901293,0.00048650577,0.0002944368,0.00022729245,0.0014437552],"category_scores_gemma":[0.00033114475,0.00015181689,0.00035540745,0.0009658046,0.0001397437,0.00024489596,0.00054261665,0.00029395937,0.00032636547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004941219,0.0001729655,0.82063365,0.00016175228,0.0005564057,0.0015931427,0.0004057076,0.017546775,0.11822063,0.0012565497,0.007470589,0.03148781],"study_design_scores_gemma":[0.0000141216005,0.000033221088,0.9870487,0.000009753355,0.00005506036,0.00015698183,0.000053110492,0.005376528,0.0030437105,0.00014517823,0.0040461193,0.000017555687],"about_ca_topic_score_codex":0.01968376,"about_ca_topic_score_gemma":0.04806246,"teacher_disagreement_score":0.01968376,"about_ca_system_score_codex":0.00031250616,"about_ca_system_score_gemma":0.00020653075,"threshold_uncertainty_score":0.039138377},"labels":[],"label_agreement":null},{"id":"W2148547933","doi":"10.1088/0004-637x/737/1/9","title":"OBSERVATIONAL PROPERTIES OF THE METAL-POOR THICK DISK OF THE MILKY WAY AND INSIGHTS INTO ITS ORIGINS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Thick disk; Astrophysics; Stars; Physics; Milky Way; Thin disk; Galaxy; Accretion (finance); Giant star; Astronomy; Population; Halo","score_opus":0.045250207060165325,"score_gpt":0.23014958577569003,"score_spread":0.1848993787155247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148547933","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942636,0.00010855354,0.000071449,0.000011648365,5.397256e-7,0.0000017865085,0.00012230636,0.000002073323,0.0002553721],"genre_scores_gemma":[0.9991037,0.00011282083,0.00022370247,0.000008836481,0.0000044607077,0.0000029227015,0.00037753882,0.000003846834,0.00016225853],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997428,0.000051347477,0.000028636223,0.00008060846,0.000052934898,0.000043719774],"domain_scores_gemma":[0.9988513,0.00015986609,0.0004941535,0.00013817879,0.00017549953,0.0001809783],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005025328,0.00020686403,0.0002882638,0.0012543842,0.00045314291,0.0008793778,0.0003573007,0.00021575164,0.00048583702],"category_scores_gemma":[0.0016504003,0.0001561678,0.00014835346,0.0013539637,0.00046775944,0.0005644455,0.0008337867,0.00018255886,0.00013597641],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027579657,0.000007764369,0.99426407,0.000013375028,0.000017253542,0.000061546896,0.00023157928,0.000105336265,0.0030845068,0.00005753249,0.000021999242,0.0021074566],"study_design_scores_gemma":[0.0000011677835,0.000014541348,0.9991099,0.0000031867917,0.00000503762,0.00006499335,0.00016910196,0.00007942764,0.0002563931,0.000037295675,0.00025755254,0.0000013674454],"about_ca_topic_score_codex":0.0058671455,"about_ca_topic_score_gemma":0.010985259,"teacher_disagreement_score":0.0058671455,"about_ca_system_score_codex":0.00033326383,"about_ca_system_score_gemma":0.000204511,"threshold_uncertainty_score":0.011666},"labels":[],"label_agreement":null},{"id":"W2148667841","doi":"10.1088/0004-637x/769/1/39","title":"PS1-12sk IS A PECULIAR SUPERNOVA FROM A He-RICH PROGENITOR SYSTEM IN A BRIGHTEST CLUSTER GALAXY ENVIRONMENT","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; California Institute of Technology; National Aeronautics and Space Administration; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Galaxy; Cluster (spacecraft); Astronomy; White dwarf; Star formation; Galaxy cluster; Stars","score_opus":0.007034538115532813,"score_gpt":0.1945725754282901,"score_spread":0.18753803731275728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148667841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99817955,0.00022236219,0.00021369377,0.000017344664,0.000006762201,0.0000134875445,0.00030485936,0.00003555146,0.0010063743],"genre_scores_gemma":[0.99718636,0.00018426547,0.0003840367,0.000024108556,0.00001565402,0.0000055858154,0.0014273785,0.000009545423,0.0007630034],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999182,0.000003186263,0.000004508555,0.00002739292,0.000020425512,0.000026294294],"domain_scores_gemma":[0.99975485,0.00001096865,0.00008036273,0.000021061664,0.000017919485,0.000114934606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010358599,0.00034659906,0.00032772298,0.0005922252,0.0007810188,0.00063511496,0.0002790406,0.00023357819,0.0015797616],"category_scores_gemma":[0.00014492898,0.00013223123,0.00022824692,0.0005875606,0.00027855788,0.00019076059,0.00078187254,0.00031652985,0.00061841274],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006804511,0.00018938835,0.86657643,0.00021334157,0.0001365817,0.01040643,0.0006332862,0.00063067017,0.09432529,0.00089493534,0.001213902,0.024099272],"study_design_scores_gemma":[0.000015845728,0.0005331544,0.96754676,0.000018550814,0.00004657447,0.013990984,0.00035046678,0.00049721246,0.007636403,0.0002750651,0.009072324,0.000016588816],"about_ca_topic_score_codex":0.0031698383,"about_ca_topic_score_gemma":0.0060829967,"teacher_disagreement_score":0.0031698383,"about_ca_system_score_codex":0.00023587367,"about_ca_system_score_gemma":0.000255146,"threshold_uncertainty_score":0.006302774},"labels":[],"label_agreement":null},{"id":"W2148939953","doi":"10.1088/0004-637x/741/2/97","title":"THE FIRST SYSTEMATIC STUDY OF TYPE Ibc SUPERNOVA MULTI-BAND LIGHT CURVES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":424,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Supernova; Photometry (optics); Physics; Light curve; Astrophysics; Absolute magnitude; Luminosity; Galaxy; Extinction (optical mineralogy); Population; Astronomy; Stars; Optics","score_opus":0.02656333207947274,"score_gpt":0.24020922462626865,"score_spread":0.21364589254679592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2148939953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9842152,0.001362878,0.005392318,0.00002794218,0.000023998997,0.00007122864,0.0042462815,0.00028327163,0.004376751],"genre_scores_gemma":[0.98747766,0.00038835205,0.005026819,0.00003241631,0.000027212898,0.000042839016,0.006377437,0.000076907534,0.0005503241],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991036,0.00010148563,0.000117539166,0.00031337742,0.0002673089,0.000096718846],"domain_scores_gemma":[0.99298495,0.00069555466,0.0024837572,0.0015041077,0.0018482043,0.0004835163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010515127,0.0004546727,0.0003618187,0.0055526257,0.00055970426,0.0007828865,0.0006424084,0.00024317467,0.00070442987],"category_scores_gemma":[0.0037990003,0.0002345702,0.00043205675,0.0032181311,0.0002810144,0.0005037779,0.0011723071,0.000251987,0.00044028193],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023256438,0.000014595887,0.981602,0.000029164072,0.00009550938,0.000028700591,0.000069367496,0.00021828772,0.0026764385,0.00008705588,0.00030116466,0.014854364],"study_design_scores_gemma":[9.016744e-7,0.000025129762,0.99695647,0.000008149326,0.000026697608,0.00020239846,0.000049785078,0.000426188,0.0008624252,0.000036528072,0.0013997816,0.0000054855655],"about_ca_topic_score_codex":0.007974807,"about_ca_topic_score_gemma":0.021942379,"teacher_disagreement_score":0.007974807,"about_ca_system_score_codex":0.0005674095,"about_ca_system_score_gemma":0.0005661959,"threshold_uncertainty_score":0.015856743},"labels":[],"label_agreement":null},{"id":"W2149001020","doi":"10.1086/592244","title":"VERITAS Discovery of &gt;200 GeV Gamma-Ray Emission from the Intermediate-Frequency-Peaked BL Lacertae Object W Comae","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; BL Lac object; Crab Nebula; Astrophysics; Flare; Gamma ray; Jet (fluid); Spectral index; Flux (metallurgy); Photon; Spectral energy distribution; Astronomy; Spectral line; Blazar; Galaxy; Optics","score_opus":0.009315957367605914,"score_gpt":0.21181460936416516,"score_spread":0.20249865199655925,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149001020","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9886381,0.0005191214,0.0014575757,0.00023414618,0.000030650473,0.000013890118,0.00035494598,0.00017739007,0.008574201],"genre_scores_gemma":[0.9979499,0.00007466368,0.0006964935,0.00008779788,0.000021327278,0.0000029285893,0.0002470079,0.000010853793,0.00090911204],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998915,0.0000061336987,0.000003501261,0.00003087241,0.00002876939,0.000039313458],"domain_scores_gemma":[0.9996419,0.000050944927,0.00010939691,0.00006915334,0.000037565867,0.00009109866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025681147,0.00023315742,0.00014600214,0.0005935995,0.00044180956,0.0010390057,0.00040850998,0.00043771876,0.0027269272],"category_scores_gemma":[0.0005732706,0.0001607362,0.00017489269,0.00042814438,0.00040258924,0.00032247248,0.00066644786,0.00040762732,0.00048037578],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000990808,0.00016666077,0.50054014,0.00024211241,0.0002275692,0.008263957,0.0010543335,0.0007808787,0.41915014,0.006628069,0.0029187487,0.059036613],"study_design_scores_gemma":[0.000043647746,0.00028581725,0.9396481,0.000024675493,0.000084868254,0.0042087506,0.00028671598,0.0010587424,0.036286656,0.0016885869,0.016354432,0.000028953007],"about_ca_topic_score_codex":0.0010162799,"about_ca_topic_score_gemma":0.0013634968,"teacher_disagreement_score":0.0027269272,"about_ca_system_score_codex":0.0002298606,"about_ca_system_score_gemma":0.00011510733,"threshold_uncertainty_score":0.009122431},"labels":[],"label_agreement":null},{"id":"W2149053837","doi":"10.1088/0004-637x/805/2/179","title":"THE EVENT HORIZON OF M87","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Army Research Office; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; National Aeronautics and Space Administration; California Institute of Technology; Gordon and Betty Moore Foundation; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Event horizon; Supermassive black hole; Black hole (networking); Accretion (finance); Active galactic nucleus; Intermediate-mass black hole; Jet (fluid); Spin-flip; Accretion disc","score_opus":0.018942598651780322,"score_gpt":0.25047462290981104,"score_spread":0.2315320242580307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149053837","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9722587,0.00067058875,0.00041371927,0.0005178297,0.000015758655,0.0000075818953,0.00024218201,0.00003297272,0.025840623],"genre_scores_gemma":[0.99884605,0.000107661624,0.00008464073,0.000044749646,0.00001785702,0.0000021861345,0.00021016096,0.0000064696046,0.00068013684],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.000015323807,0.000003732979,0.000014621156,0.000027499484,0.000056547342],"domain_scores_gemma":[0.99951446,0.00008254691,0.00017166868,0.00004094666,0.00005409621,0.00013620708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002533923,0.00009594144,0.00019140264,0.00043971234,0.0007528178,0.0010480842,0.00020090298,0.00028088232,0.0021407746],"category_scores_gemma":[0.0014954155,0.00008027671,0.00010418928,0.0003598018,0.00048502407,0.00050376466,0.001011816,0.00033187988,0.00047369828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021296255,0.0002218965,0.61594653,0.00024478737,0.00009809997,0.008150212,0.014358877,0.0016085033,0.026260348,0.1785808,0.01392341,0.13847692],"study_design_scores_gemma":[0.000028117993,0.00014332552,0.95588195,0.000060974897,0.000030475308,0.0010149447,0.0017728773,0.0010523804,0.0013331732,0.017926836,0.02073804,0.00001690917],"about_ca_topic_score_codex":0.0033048543,"about_ca_topic_score_gemma":0.002443495,"teacher_disagreement_score":0.0033048543,"about_ca_system_score_codex":0.00064166065,"about_ca_system_score_gemma":0.00031812448,"threshold_uncertainty_score":0.0071615577},"labels":[],"label_agreement":null},{"id":"W2149449857","doi":"10.1088/0004-637x/783/1/16","title":"OBSERVATIONS OF THE UNIDENTIFIED GAMMA-RAY SOURCE TeV J2032+4130 BY VERITAS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Science Foundation; Science Foundation Ireland; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution","keywords":"Physics; Astrophysics; Context (archaeology); Pulsar wind nebula; Telescope; Astronomy; Nebula; Stars","score_opus":0.009618689151115422,"score_gpt":0.2020412079701444,"score_spread":0.192422518819029,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149449857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963266,0.00013498872,0.00033053118,0.000048766462,0.000009390497,0.000008492237,0.00089666725,0.000048875692,0.0021957825],"genre_scores_gemma":[0.9954917,0.000097934775,0.0010715083,0.00005485711,0.000017828477,0.000009145076,0.0024143783,0.000023422937,0.00081928296],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998153,0.000014909359,0.000006876351,0.000043855413,0.00007430321,0.000044798067],"domain_scores_gemma":[0.9996426,0.00004500811,0.000113591275,0.00005869548,0.0000366354,0.00010357529],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029947868,0.0002560992,0.0003761196,0.00087573717,0.0005074501,0.00053094607,0.0004862999,0.00043510535,0.0011101199],"category_scores_gemma":[0.00046076727,0.00029764557,0.00026668044,0.0007779114,0.00023632636,0.00026699615,0.0007995821,0.00051906635,0.0003868286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012228816,0.00021717258,0.49663946,0.00013659008,0.00023665934,0.0058284495,0.0014094408,0.001957141,0.45611492,0.00153225,0.0034692548,0.031235758],"study_design_scores_gemma":[0.00003362967,0.00012757537,0.99052984,0.000020969741,0.000034931123,0.001062629,0.00014595197,0.0013314956,0.0031594562,0.00016302844,0.0033676836,0.00002284425],"about_ca_topic_score_codex":0.0065014292,"about_ca_topic_score_gemma":0.022173546,"teacher_disagreement_score":0.0065014292,"about_ca_system_score_codex":0.00044931416,"about_ca_system_score_gemma":0.00037451755,"threshold_uncertainty_score":0.012927175},"labels":[],"label_agreement":null},{"id":"W2149470802","doi":"10.1088/0004-637x/704/2/l75","title":"PARTICLE CLUMPING AND PLANETESIMAL FORMATION DEPEND STRONGLY ON METALLICITY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":423,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planetesimal; Metallicity; Streaming instability; Physics; Particle (ecology); Astrophysics; Particle density; Exoplanet; Planet; Plasma; Geology; Galaxy","score_opus":0.014573709509088385,"score_gpt":0.2413958119963516,"score_spread":0.22682210248726323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149470802","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939032,0.000060718656,0.0021133346,0.00019678022,0.000021431493,0.000025944624,0.00023338966,0.000081133236,0.003363997],"genre_scores_gemma":[0.9973738,0.00004690127,0.0018068003,0.000041669085,0.0000059955228,0.000027206623,0.00020702022,0.000028139164,0.0004625102],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998765,0.000024049128,0.000008168707,0.000018890205,0.000027479506,0.00004483351],"domain_scores_gemma":[0.9988611,0.0006132823,0.00014754718,0.000058145582,0.00010655486,0.00021341143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031775254,0.00055270933,0.0005510902,0.00044373763,0.0009911852,0.0011603273,0.0008530144,0.0011297265,0.0018248665],"category_scores_gemma":[0.0029441589,0.0004716015,0.000570531,0.00045969375,0.0014787349,0.00068711146,0.0007213799,0.0010360053,0.0001628592],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021455625,0.00016019867,0.016757797,0.000029222545,0.000052757277,0.00022075538,0.00012197469,0.9762864,0.0025672154,0.0020084688,0.00030146388,0.0012790967],"study_design_scores_gemma":[0.00006651996,0.000043491425,0.0019733005,0.0000053037143,0.000013149108,0.000022024582,0.000050278602,0.99643695,0.00061905023,0.0005969263,0.00016215806,0.000010823044],"about_ca_topic_score_codex":0.024614753,"about_ca_topic_score_gemma":0.013594217,"teacher_disagreement_score":0.024614753,"about_ca_system_score_codex":0.0010708163,"about_ca_system_score_gemma":0.0008222986,"threshold_uncertainty_score":0.048942983},"labels":[],"label_agreement":null},{"id":"W2149496379","doi":"10.1088/0004-637x/794/2/103","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. VIII. THE SPATIAL DISTRIBUTION OF GLOBULAR CLUSTERS IN THE VIRGO CLUSTER","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Waterloo; Canadian Nautical Research Society; Herzberg Institute of Astrophysics","funders":"Canadian Space Agency; Jet Propulsion Laboratory; National Natural Science Foundation of China; Canadian Foundation for AIDS Research; Agence Nationale de la Recherche; California Institute of Technology; National Aeronautics and Space Administration; Case Western Reserve University; National Science Foundation","keywords":"Virgo Cluster; Physics; Astrophysics; Globular cluster; Astronomy; Galaxy; Galaxy cluster; Population; Cluster (spacecraft); Medicine","score_opus":0.013435769460878697,"score_gpt":0.21841388078455912,"score_spread":0.20497811132368043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149496379","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.16680314,0.0035482333,0.0008009996,0.002411899,0.00030790857,0.00028347314,0.80683833,0.0008413828,0.018164605],"genre_scores_gemma":[0.23423325,0.0016356854,0.0038593784,0.0008146484,0.00015583093,0.00047868222,0.73644865,0.00014114959,0.022232756],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9997372,0.000027144832,0.000020114981,0.000050493836,0.00009177593,0.00007327287],"domain_scores_gemma":[0.9988568,0.000051887942,0.00017806,0.00011215569,0.00036405353,0.00043710388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007236521,0.00033679177,0.00025262183,0.00465477,0.0005442851,0.00084220525,0.0009132962,0.0005032202,0.0047538914],"category_scores_gemma":[0.0014166975,0.0002169938,0.00036254877,0.0046739345,0.00017244984,0.00044383976,0.0016052924,0.00048578606,0.0023873374],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035653808,0.000091909154,0.4672336,0.0004359768,0.00025242328,0.0001765202,0.00046711523,0.00064074236,0.0020678053,0.0016941373,0.47248068,0.05410259],"study_design_scores_gemma":[0.000028691167,0.000013728742,0.92336756,0.00004899979,0.000032033662,0.00005155208,0.00018776789,0.0001519686,0.00019232243,0.00017321066,0.075744055,0.00000811105],"about_ca_topic_score_codex":0.25763935,"about_ca_topic_score_gemma":0.28925785,"teacher_disagreement_score":0.25763935,"about_ca_system_score_codex":0.001673283,"about_ca_system_score_gemma":0.0017602167,"threshold_uncertainty_score":0.51227945},"labels":[],"label_agreement":null},{"id":"W2149716536","doi":"10.1088/0004-637x/786/1/1","title":"THE MOVING GROUP TARGETS OF THE SEEDS HIGH-CONTRAST IMAGING SURVEY OF EXOPLANETS AND DISKS: RESULTS AND OBSERVATIONS FROM THE FIRST THREE YEARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Exoplanet; myr; Physics; Astrophysics; Astronomy; Planet; Brown dwarf; Contrast (vision); Geology; Chemistry","score_opus":0.011969629183135898,"score_gpt":0.19759017797778727,"score_spread":0.18562054879465137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149716536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938398,0.00064115477,0.0013417301,0.000044277855,0.000006987652,0.00002499617,0.0013147627,0.00006611893,0.0027202317],"genre_scores_gemma":[0.9866881,0.00041083776,0.006164824,0.000060432823,0.00002864653,0.000028028098,0.005351857,0.000050965304,0.0012163415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997383,0.000019856536,0.000014309221,0.00005962437,0.000109699686,0.00005826406],"domain_scores_gemma":[0.99934536,0.00004804454,0.00017811534,0.00007029434,0.00014960342,0.00020857899],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045069738,0.0003498416,0.00025454463,0.0013086507,0.00039989295,0.00046694177,0.00030385685,0.0001984669,0.00046173017],"category_scores_gemma":[0.00045765608,0.00020908513,0.00027035462,0.00087329483,0.00019159474,0.0003830726,0.0008581647,0.00023066986,0.0002984503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022066028,0.00007847966,0.9283066,0.000085017775,0.00009206018,0.00036140945,0.0008140248,0.00071039854,0.0304485,0.00034404348,0.0018202311,0.036718585],"study_design_scores_gemma":[0.0000048275633,0.000062215135,0.9924407,0.000010843244,0.000025217765,0.00029202597,0.00012204374,0.00037875542,0.0026580612,0.000053071835,0.0039435336,0.000008622336],"about_ca_topic_score_codex":0.0079086,"about_ca_topic_score_gemma":0.021118497,"teacher_disagreement_score":0.0079086,"about_ca_system_score_codex":0.0004277136,"about_ca_system_score_gemma":0.00025079146,"threshold_uncertainty_score":0.015725136},"labels":[],"label_agreement":null},{"id":"W2149736976","doi":"10.1088/0004-637x/712/2/1049","title":"THE EFFECT OF PROJECTION ON DERIVED MASS-SIZE AND LINEWIDTH-SIZE RELATIONSHIPS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Virial theorem; Projection (relational algebra); Power law; Cube (algebra); Molecular cloud; Gravitational collapse; Scale (ratio); Monte Carlo method","score_opus":0.00809022783625793,"score_gpt":0.2376151055487389,"score_spread":0.22952487771248098,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149736976","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88694453,0.00048303037,0.10349195,0.0003458277,0.00005956116,0.00006154274,0.0010246208,0.0026987726,0.004890254],"genre_scores_gemma":[0.9847402,0.00009013382,0.01389483,0.00007701881,0.000007719489,0.000021617143,0.0007013643,0.0003593688,0.00010773777],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986608,0.0004563983,0.00008618669,0.00028234613,0.00040179715,0.00011243887],"domain_scores_gemma":[0.9913783,0.005556017,0.0007883077,0.0012454683,0.0008236209,0.00020835074],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028752077,0.0009383069,0.00039235433,0.0007332042,0.0004622049,0.0012756445,0.0013432226,0.00061686075,0.0009331631],"category_scores_gemma":[0.019433198,0.0005041377,0.0007365345,0.00088871096,0.0006898386,0.0016682333,0.001520714,0.001280479,0.0002882539],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027952416,0.00010954191,0.1311519,0.00020508167,0.00024106223,0.0004180764,0.00044075502,0.8058497,0.017167762,0.007139135,0.0010268694,0.0359706],"study_design_scores_gemma":[0.000029519264,0.000076729426,0.03272045,0.00004346121,0.000051137344,0.00015386735,0.00009764476,0.93797565,0.024667602,0.0030377628,0.0010847644,0.000061438885],"about_ca_topic_score_codex":0.0040586414,"about_ca_topic_score_gemma":0.00196487,"teacher_disagreement_score":0.0040586414,"about_ca_system_score_codex":0.00062306575,"about_ca_system_score_gemma":0.00069586514,"threshold_uncertainty_score":0.015205741},"labels":[],"label_agreement":null},{"id":"W2149825297","doi":"10.1088/0004-637x/744/1/40","title":"CORRELATIONS IN THE (SUB)MILLIMETER BACKGROUND FROM ACT × BLAST","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Galaxy; Astronomy; Telescope; Redshift; Cosmic background radiation; Population; Optics","score_opus":0.019903944405457553,"score_gpt":0.2164470019909945,"score_spread":0.19654305758553695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149825297","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98427933,0.000086792024,0.0066741263,0.00005773551,0.00001574989,0.000011407209,0.003240612,0.0008603829,0.004773901],"genre_scores_gemma":[0.9857934,0.000042574367,0.005558981,0.000048393988,0.000035518722,0.000013837674,0.007670519,0.00012562901,0.0007112428],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999532,0.0000392546,0.000014592928,0.00012468781,0.00020472049,0.00008481962],"domain_scores_gemma":[0.9988594,0.00023069451,0.00028870278,0.00019356135,0.0002585226,0.00016906341],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039105507,0.00034245322,0.00024623473,0.0014726929,0.00025513582,0.00067660655,0.00026868616,0.00022806114,0.0015776694],"category_scores_gemma":[0.0012412079,0.00024239247,0.00025904164,0.0015435383,0.00017255824,0.00025221007,0.00049774244,0.00032932532,0.00060055475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005634544,0.000092250746,0.843065,0.000102477425,0.00022915106,0.00059222424,0.0006578284,0.0059302375,0.08144112,0.0017813122,0.0059862784,0.059558753],"study_design_scores_gemma":[0.00000682192,0.000019480136,0.9886938,0.0000027468948,0.000019213734,0.00015733675,0.000033754164,0.0047675986,0.003937754,0.00016946498,0.0021822548,0.000009910531],"about_ca_topic_score_codex":0.0035958125,"about_ca_topic_score_gemma":0.0069100363,"teacher_disagreement_score":0.0035958125,"about_ca_system_score_codex":0.0002708216,"about_ca_system_score_gemma":0.00013093675,"threshold_uncertainty_score":0.007149756},"labels":[],"label_agreement":null},{"id":"W2149892437","doi":"10.1088/0004-637x/701/1/32","title":"GALAXY CLUSTERS DISCOVERED WITH A SUNYAEV-ZEL'DOVICH EFFECT SURVEY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":300,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"ROSAT; Galaxy cluster; Redshift; Galaxy; Sky; Declination; South Pole Telescope; Cluster (spacecraft)","score_opus":0.005741214651629089,"score_gpt":0.2120912655058237,"score_spread":0.2063500508541946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149892437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99750453,0.000106810425,0.000089373505,0.00004367751,0.0000034497739,0.00000777546,0.0004593831,0.000013936266,0.0017711243],"genre_scores_gemma":[0.9987336,0.000060667004,0.00015344414,0.000021100592,0.0000068488825,0.0000046335763,0.0006661147,0.000003554774,0.00034997007],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970406,0.000025022862,0.000013122982,0.000076106866,0.00009709535,0.00008456072],"domain_scores_gemma":[0.9992569,0.00005410301,0.00026026368,0.00006301055,0.000073248855,0.000292395],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002477598,0.00013599107,0.00022687457,0.0017374296,0.00057982805,0.00059204653,0.000218373,0.0001561523,0.0012079558],"category_scores_gemma":[0.00052518595,0.00015220405,0.000114968774,0.00080822187,0.00035339798,0.00021325587,0.0009347043,0.0002056622,0.00015689751],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004872405,0.000017079952,0.99388254,0.000007549994,0.000026288084,0.0000963584,0.00020674302,0.00007421733,0.0027589577,0.00015610813,0.000535286,0.0021901936],"study_design_scores_gemma":[0.0000024161272,0.00000833534,0.99932814,0.000001033104,0.000004083996,0.000051766387,0.000055837765,0.00003541508,0.000094990755,0.000009467318,0.00040753005,0.0000010140964],"about_ca_topic_score_codex":0.021943817,"about_ca_topic_score_gemma":0.04572291,"teacher_disagreement_score":0.021943817,"about_ca_system_score_codex":0.0006336485,"about_ca_system_score_gemma":0.00035712536,"threshold_uncertainty_score":0.04363215},"labels":[],"label_agreement":null},{"id":"W2149957750","doi":"10.1086/340498","title":"<i>Chandra</i>Observation of the Globular Cluster NGC 6440 and the Nature of Cluster X‐Ray Luminosity Functions","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Luminosity; Cluster (spacecraft); RADIUS; Observatory; Astronomy; Luminosity function; Limiting; Galaxy","score_opus":0.009233280902840266,"score_gpt":0.20058996405580998,"score_spread":0.19135668315296972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149957750","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980856,0.00013356713,0.00015114713,0.000044563727,0.0000025080212,0.00000361277,0.00033710917,0.000022901624,0.0012189111],"genre_scores_gemma":[0.99757594,0.00014708834,0.0007307056,0.000036882997,0.00001230364,0.000004078141,0.0007682152,0.00000988333,0.0007150161],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988544,0.000012377746,0.0000060351763,0.00002408423,0.000029099789,0.000042919346],"domain_scores_gemma":[0.9995521,0.000051453993,0.00015606057,0.000057608046,0.00005082544,0.00013185908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002217834,0.00014982611,0.000109297434,0.001131684,0.0004524396,0.00050527253,0.00019552324,0.00016944598,0.0013341963],"category_scores_gemma":[0.0006795229,0.00016029282,0.00009782486,0.0010897891,0.00035891435,0.0002921762,0.0004715392,0.00021973035,0.00022115475],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006410019,0.00010401427,0.83776057,0.00010401348,0.00009823279,0.0010222766,0.0008418478,0.0010032796,0.12990217,0.0012612944,0.002006763,0.025254466],"study_design_scores_gemma":[0.000008822887,0.000029718205,0.99569607,0.0000073288834,0.0000111295,0.00046650975,0.000068367226,0.00020642436,0.0020794035,0.00019649326,0.0012213583,0.000008260164],"about_ca_topic_score_codex":0.0130166365,"about_ca_topic_score_gemma":0.027206507,"teacher_disagreement_score":0.0130166365,"about_ca_system_score_codex":0.00036991056,"about_ca_system_score_gemma":0.00020095645,"threshold_uncertainty_score":0.025881767},"labels":[],"label_agreement":null},{"id":"W2149960140","doi":"10.3847/0004-637x/821/1/13","title":"THE NANOGRAV NINE-YEAR DATA SET: LIMITS ON THE ISOTROPIC STOCHASTIC GRAVITATIONAL WAVE BACKGROUND","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":328,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"Science and Technology Facilities Council; Universities Space Research Association; Associated Universities; National Science Foundation; Sherman Fairchild Foundation; Aspen Center for Physics; California Institute of Technology; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Gravitational wave; Power law; Supermassive black hole; Spectral density; Gravitational wave background; Amplitude; Law; Quantum mechanics; Galaxy; Statistics","score_opus":0.04021970511754823,"score_gpt":0.28044566506606255,"score_spread":0.2402259599485143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149960140","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.82429326,0.00061059237,0.021432426,0.0014255139,0.00020848025,0.000104151135,0.13543554,0.0018571347,0.014632866],"genre_scores_gemma":[0.75842017,0.00022544288,0.011795736,0.00032368774,0.00008847865,0.00015403074,0.2270068,0.0004473204,0.0015383718],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99866676,0.00031719825,0.00008982176,0.00028664072,0.0004921383,0.00014745406],"domain_scores_gemma":[0.99523073,0.0015021251,0.0007317579,0.0012968591,0.00082010496,0.0004182585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0039151805,0.0004922483,0.0006561152,0.0015894013,0.0006939648,0.0018086237,0.0011739228,0.0008472924,0.0035729527],"category_scores_gemma":[0.010130631,0.00038138588,0.00085667864,0.0023518596,0.00039657482,0.0010934435,0.001611823,0.0011460017,0.0016544786],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011671872,0.00034085757,0.60634804,0.00030614535,0.0007698938,0.00054523034,0.00049282884,0.24847755,0.0046975114,0.024915602,0.07628036,0.03565873],"study_design_scores_gemma":[0.0003912579,0.00011252441,0.53787535,0.00015359053,0.00014621089,0.00026162883,0.00038002318,0.3373694,0.007173558,0.018538136,0.097391546,0.00020679833],"about_ca_topic_score_codex":0.022529537,"about_ca_topic_score_gemma":0.02554641,"teacher_disagreement_score":0.022529537,"about_ca_system_score_codex":0.0007038879,"about_ca_system_score_gemma":0.0009045135,"threshold_uncertainty_score":0.044796824},"labels":[],"label_agreement":null},{"id":"W2149976538","doi":"10.1088/0004-637x/794/1/21","title":"A 24 HR GLOBAL CAMPAIGN TO ASSESS PRECISION TIMING OF THE MILLISECOND PULSAR J1713+0747","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; National Astronomical Research Institute of Thailand; Fonds Québécois de la Recherche sur la Nature et les Technologies; University of Sydney; National Science Foundation","keywords":"Pulsar; Physics; LOFAR; Scintillation; Millisecond pulsar; Noise (video); Radio telescope; Gravitational wave; Astrophysics; Astronomy; Optics; Computer science","score_opus":0.021785622026033992,"score_gpt":0.25905259035847844,"score_spread":0.23726696833244446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149976538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99463576,0.000056345725,0.0007981515,0.000025366362,0.000009374632,0.00006338014,0.0031503025,0.00005396349,0.0012072308],"genre_scores_gemma":[0.9779619,0.0001305815,0.0036712724,0.00010199749,0.000048935566,0.00027980687,0.016823618,0.00010151325,0.00088032585],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996798,0.00006843996,0.000016888105,0.000082079954,0.0000628392,0.000089930625],"domain_scores_gemma":[0.9987978,0.00013291309,0.0002588829,0.00025623944,0.00028147685,0.00027275327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006574907,0.00033910305,0.0003738195,0.00087436143,0.00044832993,0.0003492897,0.00023521631,0.00029666082,0.00094683253],"category_scores_gemma":[0.0005921885,0.00014464554,0.0002518172,0.0009794487,0.00032946758,0.00027610842,0.0006799828,0.00035758287,0.0003481607],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015773779,0.00062295754,0.8422561,0.00012578741,0.00042712712,0.00034178788,0.0011868185,0.0020428463,0.10585696,0.00040358753,0.002814615,0.042343963],"study_design_scores_gemma":[0.00003361807,0.00033848136,0.9941812,0.0000038044684,0.00004799542,0.00008416144,0.00012478388,0.00033148692,0.002944768,0.00002588154,0.0018758756,0.000007815015],"about_ca_topic_score_codex":0.010729752,"about_ca_topic_score_gemma":0.015375494,"teacher_disagreement_score":0.010729752,"about_ca_system_score_codex":0.00035219695,"about_ca_system_score_gemma":0.00056281185,"threshold_uncertainty_score":0.021334589},"labels":[],"label_agreement":null},{"id":"W2149990597","doi":"10.1088/0004-637x/727/2/129","title":"INSIGHTS INTO THE HIGH-ENERGY γ-RAY EMISSION OF MARKARIAN 501 FROM EXTENSIVE MULTIFREQUENCY OBSERVATIONS IN THE<i>FERMI</i>ERA","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":237,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Japan Aerospace Exploration Agency; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Instituto de Astrofísica de Canarias; Natural Sciences and Engineering Research Council of Canada; Istituto Nazionale di Astrofisica; Georgian National Science Foundation; Centre National de la Recherche Scientifique; Smithsonian Institution; U.S. Department of Energy; Vetenskapsrådet; Max-Planck-Gesellschaft; High Energy Accelerator Research Organization; Ministerio de Ciencia e Innovación; Bundesministerium für Bildung und Forschung; Russian Foundation for Basic Research; Academia Sinica; Istituto Nazionale di Fisica Nucleare; Deutsche Forschungsgemeinschaft; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Agenzia Spaziale Italiana; Helmholtz-Gemeinschaft; Associated Universities; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Science Foundation Ireland; National Science Foundation","keywords":"Physics; Astrophysics; Blazar; Fermi Gamma-ray Space Telescope; Spectral index; Spectral energy distribution; Synchrotron; Flux (metallurgy); Luminosity; Astronomy; Gamma ray; Photon; Active galactic nucleus; Galaxy; Spectral line; Optics","score_opus":0.018244447532833667,"score_gpt":0.21075798770129237,"score_spread":0.1925135401684587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2149990597","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985643,0.00011780939,0.0002510718,0.000021115595,0.0000012449121,0.0000017681404,0.00021408236,0.0000143984025,0.0008141948],"genre_scores_gemma":[0.99854434,0.00009913471,0.0005417526,0.000021928305,0.000008049061,0.0000024661065,0.0005955226,0.000007631387,0.00017918121],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999151,0.0000081947865,0.0000052613555,0.000025931775,0.000023280967,0.000022226042],"domain_scores_gemma":[0.9997609,0.000029925193,0.000121973564,0.000028706712,0.00002102294,0.000037513022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015972008,0.00017505919,0.0001873719,0.0007412448,0.00023557183,0.0004536925,0.00019057535,0.00019722639,0.00062577624],"category_scores_gemma":[0.00033950742,0.00014924607,0.00017287691,0.00045947055,0.00024222082,0.00029314944,0.0004056219,0.00017181433,0.00017248931],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032026868,0.00005932839,0.7802499,0.000065634784,0.00013217145,0.0007147919,0.0005851,0.0024123262,0.19087134,0.0006778407,0.00057186105,0.02333938],"study_design_scores_gemma":[0.0000019820466,0.00001767755,0.9968412,0.000004267337,0.000014187457,0.0001616171,0.000053222735,0.0004978706,0.0017666818,0.000048645943,0.0005875792,0.0000049636324],"about_ca_topic_score_codex":0.005012783,"about_ca_topic_score_gemma":0.013906918,"teacher_disagreement_score":0.005012783,"about_ca_system_score_codex":0.0004148451,"about_ca_system_score_gemma":0.000114614886,"threshold_uncertainty_score":0.009967208},"labels":[],"label_agreement":null},{"id":"W2150060776","doi":"10.1086/338841","title":"Positron Abundance in Galactic Cosmic Rays","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Cosmic ray; Positron; PAMELA detector; Astrophysics; Electron; Solar wind; Astronomy; Heliosphere; Antimatter; Ultra-high-energy cosmic ray; Nuclear physics; Plasma","score_opus":0.0077347813224968994,"score_gpt":0.21171207245079957,"score_spread":0.20397729112830268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150060776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973122,0.00020194576,0.000033396656,0.000042586118,0.0000040242335,0.0000022229929,0.00044701624,0.0000034949414,0.0019530825],"genre_scores_gemma":[0.99639076,0.000273409,0.00008815131,0.00002549377,0.0000038400008,0.000003673388,0.0010882982,0.0000037562775,0.0021226404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999962,0.000007137723,0.0000014916858,0.000007696212,0.000011276648,0.000010364766],"domain_scores_gemma":[0.9998124,0.000012322218,0.00003575509,0.000011257793,0.0000768378,0.000051389266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010047007,0.0001486239,0.00014949476,0.0007097749,0.0004063768,0.00055261585,0.0001834444,0.00012656457,0.0013267082],"category_scores_gemma":[0.00043746157,0.00010494971,0.00005116764,0.00059585867,0.00025028817,0.00013912877,0.00026337715,0.00020566591,0.00018270827],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015915732,0.000023519695,0.9819952,0.000013448488,0.000028070519,0.00012560423,0.00027118562,0.00010184903,0.012923275,0.00030227995,0.00037385497,0.0036825028],"study_design_scores_gemma":[0.0000042046818,0.000025643758,0.99629104,0.000006034202,0.0000073382157,0.00007885767,0.00022844266,0.000111571404,0.0013464474,0.00005316582,0.001844378,0.0000030189535],"about_ca_topic_score_codex":0.104333065,"about_ca_topic_score_gemma":0.26654172,"teacher_disagreement_score":0.104333065,"about_ca_system_score_codex":0.00085469853,"about_ca_system_score_gemma":0.00036252043,"threshold_uncertainty_score":0.20745158},"labels":[],"label_agreement":null},{"id":"W2150108369","doi":"10.1088/0004-637x/709/1/97","title":"A WEAK LENSING STUDY OF X-RAY GROUPS IN THE COSMOS SURVEY: FORM AND EVOLUTION OF THE MASS-LUMINOSITY RELATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":289,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Waterloo","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Lawrence Berkeley National Laboratory; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; California Institute of Technology; National Aeronautics and Space Administration; Agence Nationale de la Recherche; European Southern Observatory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Halo; Weak gravitational lensing; Redshift; Luminosity; Gravitational lens; Galaxy; Galaxy cluster; Power law; Luminosity function; Intracluster medium; Astronomy","score_opus":0.01085690870205562,"score_gpt":0.21688955245703756,"score_spread":0.20603264375498193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150108369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917597,0.00004999718,0.0002688413,0.000015882337,4.6725452e-7,0.0000018454632,0.00007243767,0.000003876805,0.00041071177],"genre_scores_gemma":[0.9993432,0.000049436778,0.0003349387,0.00000569469,0.0000022967981,0.0000016642466,0.00013406014,0.000002476369,0.0001261268],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987984,0.00003155011,0.000008860668,0.00003537308,0.000024138591,0.000020204046],"domain_scores_gemma":[0.9992003,0.000145018,0.00035260338,0.00009671445,0.000071132294,0.00013432006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033175587,0.00024844887,0.00015900178,0.001109081,0.00036009072,0.0005373701,0.0001368966,0.0001257624,0.0007345491],"category_scores_gemma":[0.001347497,0.00011112763,0.00019260655,0.00073941686,0.00035695927,0.0004681466,0.0007383019,0.00021338808,0.00022148989],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000017590917,0.0000068642416,0.9948255,0.0000040384634,0.000018736046,0.000018490517,0.00009924278,0.00013931264,0.0025177218,0.00016288835,0.000023365466,0.0021663771],"study_design_scores_gemma":[9.130925e-7,0.000022315306,0.9982799,0.0000015617694,0.00000521733,0.0000619862,0.00013446677,0.0006186947,0.000541398,0.0001450224,0.00018687619,0.0000016312958],"about_ca_topic_score_codex":0.0031082206,"about_ca_topic_score_gemma":0.0050435495,"teacher_disagreement_score":0.0031082206,"about_ca_system_score_codex":0.00017364511,"about_ca_system_score_gemma":0.00011267815,"threshold_uncertainty_score":0.0061802864},"labels":[],"label_agreement":null},{"id":"W2150120374","doi":"10.1086/426813","title":"The Double Pulsar System J0737-3039: Modulation of A by B at Eclipse","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Pulsar; Eclipse; Physics; Magnetosphere; Line-of-sight; Astrophysics; Plasma; Astronomy; Millisecond pulsar; Flux (metallurgy); Line (geometry); Asymmetry; Nuclear physics; Geometry","score_opus":0.009620438470026247,"score_gpt":0.28878580746811683,"score_spread":0.2791653689980906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150120374","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994311,0.000047272802,0.000052101,0.000006222826,0.000001731791,0.0000015711187,0.00008735233,0.000004115363,0.00036844544],"genre_scores_gemma":[0.9995528,0.000023352633,0.00010580683,0.0000067838173,0.0000029325995,0.0000028307275,0.00020483782,0.0000032787382,0.00009734302],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999223,0.0000066614343,0.000003982966,0.000022915363,0.000017698181,0.000026611837],"domain_scores_gemma":[0.99971646,0.000046928828,0.000081631355,0.00002519998,0.000052517316,0.00007724921],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010475264,0.00016108726,0.0003249271,0.0005980454,0.00036242936,0.0003220399,0.00015061953,0.00025402097,0.0006078334],"category_scores_gemma":[0.00036011852,0.00015365086,0.00010998559,0.0004953114,0.00024514523,0.00020402098,0.0003777119,0.00025742457,0.00025445488],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008724774,0.00008187741,0.3691233,0.000058514364,0.00006252359,0.0011088445,0.00048690592,0.00043290228,0.6180037,0.00021796931,0.00031332296,0.009237604],"study_design_scores_gemma":[0.000015670621,0.00011921939,0.989302,0.0000050097306,0.000013412923,0.0006369477,0.00012323547,0.0007714513,0.00829588,0.000059750135,0.00064929266,0.000008101253],"about_ca_topic_score_codex":0.0039924164,"about_ca_topic_score_gemma":0.0083319405,"teacher_disagreement_score":0.0039924164,"about_ca_system_score_codex":0.00027339932,"about_ca_system_score_gemma":0.00017908294,"threshold_uncertainty_score":0.007938325},"labels":[],"label_agreement":null},{"id":"W2150172268","doi":"10.1088/0004-637x/803/2/82","title":"DISCOVERY OF TWO NEW THERMALLY BLOATED LOW-MASS WHITE DWARFS AMONG THE<i>KEPLER</i>BINARIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"White dwarf; Radial velocity; Stars; Kepler; Star (game theory); Orbital elements; Binary star; Degenerate energy levels","score_opus":0.012819090015806844,"score_gpt":0.22444401419391313,"score_spread":0.2116249241781063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150172268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995345,0.00006632388,0.00007547168,0.000007852721,0.0000020291563,0.0000020717112,0.000046571713,0.0000041253265,0.00026111677],"genre_scores_gemma":[0.9990977,0.000050701718,0.00023982536,0.00001709763,0.000005921407,0.0000030304102,0.00031636,0.0000029999646,0.00026628884],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982846,0.000008255958,0.000016149143,0.00007047227,0.000040086048,0.00003667906],"domain_scores_gemma":[0.99951327,0.000045851728,0.00021437924,0.000041201456,0.000043373475,0.00014195096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016270195,0.00022537594,0.0002996489,0.0011619803,0.00082560757,0.0011217224,0.00030027004,0.00031981006,0.0005390183],"category_scores_gemma":[0.00044354307,0.00022085135,0.00012359984,0.0007288265,0.0004618061,0.00042063356,0.00072329014,0.0003788569,0.00027626744],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032302935,0.00006831123,0.8763252,0.000037321,0.000053246367,0.0010710527,0.0009067404,0.00016914448,0.1084144,0.00035554753,0.00022814752,0.012047861],"study_design_scores_gemma":[0.000015142896,0.00009865974,0.98931676,0.000005222714,0.00002673878,0.001552203,0.0002275822,0.00024661748,0.006720991,0.00012641067,0.0016502618,0.000013277506],"about_ca_topic_score_codex":0.0017977144,"about_ca_topic_score_gemma":0.0037252023,"teacher_disagreement_score":0.0017977144,"about_ca_system_score_codex":0.00043456425,"about_ca_system_score_gemma":0.00018591103,"threshold_uncertainty_score":0.0035745502},"labels":[],"label_agreement":null},{"id":"W2150222923","doi":"10.1088/0004-637x/807/1/93","title":"DEEP<i>NuSTAR</i>AND<i>SWIFT</i>MONITORING OBSERVATIONS OF THE MAGNETAR 1E 1841−045","year":2015,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Fonds Québécois de la Recherche sur la Nature et les Technologies; National Aeronautics and Space Administration; California Institute of Technology; Canada Research Chairs; Canadian Institute for Advanced Research","keywords":"Physics; Magnetar; Swift; Astrophysics; Astronomy; Neutron star","score_opus":0.040142632890792666,"score_gpt":0.3097766884887649,"score_spread":0.2696340555979722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150222923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99686,0.00018808708,0.00054841384,0.00005202027,0.000013860626,0.000008686473,0.0006559168,0.00007865726,0.0015943332],"genre_scores_gemma":[0.99517053,0.00010073467,0.0020811402,0.00006408143,0.000029984794,0.000009155797,0.0018838696,0.000018867975,0.0006416063],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987996,0.000009429975,0.00000563104,0.000036430018,0.00003688898,0.000031726468],"domain_scores_gemma":[0.99974746,0.000013483453,0.00010649839,0.000023697214,0.000041021955,0.00006784825],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002967434,0.00023180175,0.0003692667,0.0006691942,0.0003913812,0.00038218877,0.00031642785,0.00036001523,0.00052586873],"category_scores_gemma":[0.00032185757,0.00021577858,0.00025950142,0.00038915637,0.00020153383,0.00023934593,0.00060404575,0.00034665887,0.00027095125],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082836364,0.00032055756,0.7187128,0.00022359955,0.00031139498,0.001911304,0.00083356193,0.002890762,0.23162413,0.00044688786,0.0035198978,0.038376726],"study_design_scores_gemma":[0.000014144563,0.00017443109,0.99176425,0.000010309445,0.00003515403,0.00044550182,0.00007879692,0.0012152906,0.0032892334,0.000072987146,0.0028840438,0.00001592199],"about_ca_topic_score_codex":0.002563914,"about_ca_topic_score_gemma":0.010203259,"teacher_disagreement_score":0.002563914,"about_ca_system_score_codex":0.00033990364,"about_ca_system_score_gemma":0.00021341779,"threshold_uncertainty_score":0.0050979257},"labels":[],"label_agreement":null},{"id":"W2150238988","doi":"10.1088/0004-637x/800/2/135","title":"THE MASS OF Kepler-93b AND THE COMPOSITION OF TERRESTRIAL PLANETS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":228,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Université de Genève; Queen's University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Scottish Universities Physics Alliance; University of St Andrews; Queen's University Belfast; European Commission; John Templeton Foundation; Fundação para a Ciência e a Tecnologia; Harvard University; Smithsonian Institution; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Planet; Terrestrial planet; Planetary mass; Radial velocity; RADIUS; Exoplanet; Population; Planetary system","score_opus":0.015277587091569397,"score_gpt":0.22777368424416966,"score_spread":0.21249609715260026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150238988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98934585,0.0011575456,0.0005148625,0.000059626524,0.00000524125,0.000007718266,0.0019266502,0.000031863896,0.0069507174],"genre_scores_gemma":[0.996219,0.00026638492,0.00062011706,0.000014132271,0.0000071965574,0.0000051749016,0.0021631045,0.000016124959,0.0006887772],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986446,0.000013588423,0.000010330441,0.00005941675,0.000032000768,0.000020188],"domain_scores_gemma":[0.99949884,0.0000590918,0.0002703987,0.000044132656,0.000040087627,0.00008753438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014005839,0.00029581212,0.00023597355,0.0013596028,0.00034429049,0.0008358295,0.00025912366,0.00030018188,0.0025484653],"category_scores_gemma":[0.0011833552,0.00016192858,0.00017858214,0.0011377572,0.00029892157,0.0006096076,0.00082982995,0.00024394445,0.0013014792],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051410624,0.000027016715,0.9628346,0.000089077184,0.00012119592,0.00030526705,0.00055643835,0.00072539266,0.015685556,0.0014462819,0.0009334038,0.016761681],"study_design_scores_gemma":[0.0000050645035,0.000024259129,0.9941702,0.00001278103,0.000012213913,0.0005081701,0.000121213314,0.0004476983,0.0009030181,0.00038867968,0.0034006934,0.000006098904],"about_ca_topic_score_codex":0.002769684,"about_ca_topic_score_gemma":0.0024530326,"teacher_disagreement_score":0.002769684,"about_ca_system_score_codex":0.00037835573,"about_ca_system_score_gemma":0.00009561393,"threshold_uncertainty_score":0.008525431},"labels":[],"label_agreement":null},{"id":"W2150269717","doi":"10.1086/512055","title":"A Multiwavelength Study of 1WGA J1346.5−6255: A New γ Cas Analog Unrelated to the Background Supernova Remnant G309.2−00.6","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"ROSAT; Physics; Astrophysics; Supernova remnant; Nebula; Supernova; Astronomy; Flux (metallurgy); Star (game theory); Stars; Galaxy","score_opus":0.02919526348338676,"score_gpt":0.27994514333677956,"score_spread":0.2507498798533928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150269717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99944097,0.00003952542,0.000023269484,0.000009616309,0.0000014165172,0.0000039002384,0.000064743566,0.000002338134,0.00041413543],"genre_scores_gemma":[0.99892765,0.00005059615,0.00015718363,0.000026522486,0.0000065875033,0.0000030968133,0.00032213776,0.0000037366385,0.00050251983],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999324,0.0000042846787,0.0000038599583,0.000021932607,0.00001323386,0.00002435071],"domain_scores_gemma":[0.999843,0.000008639523,0.000047412996,0.0000112676325,0.000012251994,0.00007732938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008700203,0.00021362462,0.00021554047,0.0007340183,0.0005534867,0.00035449682,0.00019492797,0.00020212482,0.0009751776],"category_scores_gemma":[0.00013806004,0.00012564145,0.00022873077,0.000335159,0.00022272769,0.00019272229,0.00039262732,0.00026614475,0.00023745319],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061825506,0.00052314537,0.7233442,0.00007022595,0.00013271462,0.006228199,0.0011183629,0.00019879322,0.2532684,0.00041664118,0.00044779712,0.0136333],"study_design_scores_gemma":[0.000002826096,0.00008322276,0.99782515,0.0000023696925,0.000009712376,0.000781235,0.00014080513,0.000050904844,0.0006680129,0.000013412184,0.0004197642,0.0000026173084],"about_ca_topic_score_codex":0.010293964,"about_ca_topic_score_gemma":0.019187355,"teacher_disagreement_score":0.010293964,"about_ca_system_score_codex":0.00033042702,"about_ca_system_score_gemma":0.000110632696,"threshold_uncertainty_score":0.020468116},"labels":[],"label_agreement":null},{"id":"W2150347585","doi":"10.1086/312518","title":"A Definitive Optical Detection of a Supercluster at [CLC][ITAL]z[/ITAL][/CLC] ≈ 0.91","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Astrophysics; Physics; Redshift; Supercluster (genetic); Galaxy; Sky; Astronomy; Population; Cluster (spacecraft); Chemistry","score_opus":0.006491574711949919,"score_gpt":0.19588521642017584,"score_spread":0.18939364170822592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150347585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99026054,0.00013325892,0.0006325146,0.00009299202,0.000014321042,0.00001760613,0.0007846124,0.00010976162,0.007954379],"genre_scores_gemma":[0.99637234,0.0000332417,0.0009322897,0.000046393132,0.000012281437,0.0000075377093,0.0013442971,0.000012834152,0.001238831],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998522,0.00000444648,0.0000072341913,0.000035041314,0.000057407357,0.000043637207],"domain_scores_gemma":[0.9991372,0.000058430072,0.00026089523,0.00008336614,0.00018974181,0.00027047336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018118386,0.00014916867,0.00015427245,0.0006723147,0.00036069902,0.0007201408,0.00038275684,0.00024563726,0.004827856],"category_scores_gemma":[0.000663938,0.00011719873,0.00009138213,0.00045285813,0.00029106354,0.0002215974,0.0004841575,0.00024233632,0.0007818103],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003426169,0.000075265954,0.74460214,0.00007476682,0.00007908835,0.00068994355,0.00026895409,0.0004123037,0.22189902,0.0020043598,0.0033939213,0.026157567],"study_design_scores_gemma":[0.00002809728,0.000100903606,0.9680893,0.000015263731,0.000028207785,0.0006832922,0.00017001838,0.0013159252,0.019210732,0.00063093245,0.009713268,0.000014063136],"about_ca_topic_score_codex":0.0031305486,"about_ca_topic_score_gemma":0.0036252749,"teacher_disagreement_score":0.004827856,"about_ca_system_score_codex":0.0003198317,"about_ca_system_score_gemma":0.00019891514,"threshold_uncertainty_score":0.016150773},"labels":[],"label_agreement":null},{"id":"W2150450660","doi":"10.1088/0004-637x/742/2/97","title":"A<i>CHANDRA</i>X-RAY OBSERVATION OF THE BINARY MILLISECOND PULSAR PSR J1023+0038","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; Smithsonian Astrophysical Observatory; Killam Trusts; Fonds Québécois de la Recherche sur la Nature et les Technologies; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; West Virginia University; Smithsonian Institution","keywords":"Physics; Pulsar; Astrophysics; Millisecond pulsar; Binary pulsar; Astronomy; Pulsar wind nebula; Luminosity; Neutron star; Nebula; X-ray pulsar; Orbital plane; Pulsar planet; Stars; Galaxy","score_opus":0.026986037015783605,"score_gpt":0.21876910413914022,"score_spread":0.1917830671233566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150450660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98962563,0.00036811974,0.00034171215,0.0001329116,0.000020709185,0.00003720887,0.0016306965,0.0001823007,0.007660722],"genre_scores_gemma":[0.99246806,0.0002572884,0.0029856125,0.0001336667,0.000057928904,0.000031051262,0.0025516532,0.00003409127,0.0014806694],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992335,0.000003915772,0.0000043237333,0.00001603982,0.000025252135,0.000027132546],"domain_scores_gemma":[0.99979526,0.000016166448,0.00006238338,0.000033031836,0.00002446274,0.000068778434],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011359787,0.00024938036,0.00021391835,0.0010110216,0.00045080134,0.0004531518,0.00035845884,0.00027674594,0.0025046708],"category_scores_gemma":[0.00025585855,0.00016100574,0.0001742392,0.0007697197,0.00015673945,0.00028945654,0.00043906693,0.00034087052,0.00045618822],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018830587,0.00066460867,0.28806567,0.00048229244,0.00025045342,0.0053159622,0.0006097245,0.001518853,0.6276235,0.0012161235,0.009203664,0.06316614],"study_design_scores_gemma":[0.00006742379,0.00030304978,0.9701845,0.000032008484,0.000054417786,0.004939821,0.00013946879,0.0011389572,0.014756297,0.0002975581,0.008059055,0.000027504182],"about_ca_topic_score_codex":0.0039942088,"about_ca_topic_score_gemma":0.0077571846,"teacher_disagreement_score":0.0039942088,"about_ca_system_score_codex":0.00027358287,"about_ca_system_score_gemma":0.00025688394,"threshold_uncertainty_score":0.008378983},"labels":[],"label_agreement":null},{"id":"W2150493261","doi":"10.1088/0004-637x/697/2/l91","title":"DISCOVERY OF THE FIRST RETROGRADE TRANSNEPTUNIAN OBJECT","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Neptune; Trans-Neptunian object; Astronomy; Astrometry; Orbit (dynamics); Uranus; Nice model; Solar System; Telescope; Astrophysics; Planet; Planetary system; Aerospace engineering; Stars; Planetary migration","score_opus":0.005912217710837755,"score_gpt":0.19602955626061844,"score_spread":0.1901173385497807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150493261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.85985774,0.0028733886,0.013050075,0.0050760494,0.0013044052,0.00008770174,0.0013094911,0.0005349627,0.11590611],"genre_scores_gemma":[0.9606713,0.00081322325,0.008499549,0.0008432331,0.00037747156,0.000027359494,0.0013159325,0.00008853206,0.027363451],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998418,0.0000066836024,0.0000056660497,0.00007353299,0.000038056187,0.00003421885],"domain_scores_gemma":[0.9996779,0.00004559936,0.000046409197,0.000109395536,0.000050395593,0.00007037329],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050157524,0.0004301555,0.00044049518,0.0006556126,0.0013696691,0.002429841,0.00063200976,0.0026449428,0.006590349],"category_scores_gemma":[0.0008074528,0.00030264977,0.0006240065,0.0005796023,0.0007273139,0.0013694832,0.0017318124,0.0017080161,0.0027373494],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002651375,0.0002441378,0.0839846,0.0008447398,0.00025070368,0.040547173,0.0027576657,0.0017591816,0.5697679,0.090237625,0.015501963,0.191453],"study_design_scores_gemma":[0.0001968207,0.0015073959,0.20739342,0.00022527375,0.00031975043,0.048341844,0.0024070644,0.0034229036,0.14756839,0.018042848,0.5703875,0.00018687661],"about_ca_topic_score_codex":0.00075749645,"about_ca_topic_score_gemma":0.000715378,"teacher_disagreement_score":0.006590349,"about_ca_system_score_codex":0.0007613327,"about_ca_system_score_gemma":0.00047044127,"threshold_uncertainty_score":0.022046864},"labels":[],"label_agreement":null},{"id":"W2150520267","doi":"10.1088/0004-637x/812/1/81","title":"ARECIBO PULSAR SURVEY USING ALFA. IV. MOCK SPECTROMETER DATA ANALYSIS, SURVEY SENSITIVITY, AND THE DISCOVERY OF 40 PULSARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Office of Naval Research; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Canada Research Chairs; Natural Sciences and Engineering Research Council of Canada; European Commission; Universities Space Research Association; National Science Foundation; Compute Canada; Canarie; Science and Technology Facilities Council; Fonds Québécois de la Recherche sur la Nature et les Technologies; McGill University; Canadian Institute for Advanced Research","keywords":"Pulsar; Sensitivity (control systems); Physics; Astronomy; Spectrometer; Survey research; Remote sensing; Astrophysics; Geology; Engineering; Optics; Psychology","score_opus":0.0819564584383629,"score_gpt":0.3648749565056674,"score_spread":0.2829184980673045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150520267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9800014,0.0001014889,0.010672733,0.00009337174,0.000015822136,0.00008544137,0.0029298656,0.0011122823,0.0049877088],"genre_scores_gemma":[0.9634322,0.00009547373,0.025579067,0.00008285872,0.00002394102,0.000107335814,0.009018232,0.000119627395,0.0015413368],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970394,0.00006515453,0.00001205932,0.00006708647,0.00011257897,0.00003916364],"domain_scores_gemma":[0.9993716,0.000105223786,0.00016153288,0.00013323904,0.00017232088,0.000056180343],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007326171,0.0003830693,0.00022757566,0.001019579,0.00039528304,0.0004231149,0.00028360606,0.00021838548,0.00075664086],"category_scores_gemma":[0.0014907484,0.00023069384,0.00034786572,0.000771162,0.00020676877,0.00018346136,0.00032588912,0.00014951572,0.00032842517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087178306,0.00016639697,0.79349554,0.00010962283,0.00020038735,0.00028005388,0.00046661805,0.01837268,0.05874443,0.001925064,0.0070634973,0.11830393],"study_design_scores_gemma":[0.000039797407,0.000103950944,0.95582914,0.000011808828,0.0000397817,0.000163721,0.00007276614,0.026198983,0.009665142,0.0005228785,0.0073283957,0.000023613344],"about_ca_topic_score_codex":0.018503428,"about_ca_topic_score_gemma":0.01516914,"teacher_disagreement_score":0.018503428,"about_ca_system_score_codex":0.00061612244,"about_ca_system_score_gemma":0.0003407206,"threshold_uncertainty_score":0.036791444},"labels":[],"label_agreement":null},{"id":"W2150772486","doi":"10.1086/517931","title":"The All-Wavelength Extended Groth Strip International Survey (AEGIS) Data Sets","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":593,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Sky; Spectrograph; Galaxy; Infrared; Spitzer Space Telescope; Astronomy; Astrophysics; Telescope; Near-infrared spectroscopy; Optics; Spectral line","score_opus":0.029809188547341672,"score_gpt":0.27929282837804126,"score_spread":0.2494836398306996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150772486","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07653102,0.003991445,0.0025611708,0.0044619036,0.0015527696,0.0001242113,0.86399317,0.0011180054,0.045666322],"genre_scores_gemma":[0.1356646,0.003596095,0.008795925,0.0007134437,0.00051803,0.00014951512,0.82406634,0.00047527155,0.026020814],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9996431,0.00005173226,0.000031296033,0.00008758819,0.0001491778,0.000037002523],"domain_scores_gemma":[0.9986712,0.00013504545,0.00027052878,0.0002849266,0.0005301037,0.00010828031],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076146115,0.00042438894,0.00035293793,0.00456954,0.0005063342,0.0010393878,0.0007575236,0.00033098724,0.010325277],"category_scores_gemma":[0.0026492947,0.0003021925,0.00039944437,0.007080403,0.00029389438,0.00088364177,0.0010816529,0.00067180966,0.0076874876],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014569797,0.000051566483,0.11568913,0.00046705853,0.00028007364,0.00015818834,0.00026606777,0.0021110966,0.0015652613,0.00188913,0.7685525,0.10882429],"study_design_scores_gemma":[0.00004433454,0.000018524033,0.31174725,0.0003195274,0.000089394474,0.0001138394,0.00047252077,0.0013231981,0.0007711193,0.0009966557,0.68407595,0.0000277017],"about_ca_topic_score_codex":0.03954346,"about_ca_topic_score_gemma":0.08483864,"teacher_disagreement_score":0.03954346,"about_ca_system_score_codex":0.0006716234,"about_ca_system_score_gemma":0.0012198478,"threshold_uncertainty_score":0.07862657},"labels":[],"label_agreement":null},{"id":"W2150780877","doi":"10.1088/0004-637x/719/1/763","title":"EXTRAGALACTIC MILLIMETER-WAVE SOURCES IN SOUTH POLE TELESCOPE SURVEY DATA: SOURCE COUNTS, CATALOG, AND STATISTICS FOR AN 87 SQUARE-DEGREE FIELD","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":335,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Canadian Space Agency; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Kavli Institute for Cosmological Physics, University of Chicago; Jet Propulsion Laboratory; Commonwealth Scientific and Industrial Research Organisation; McGill University; Office of Polar Programs; Gordon and Betty Moore Foundation; W. M. Keck Foundation; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Source counts; Astronomy; Jansky; Population; Galaxy; Synchrotron; Flux (metallurgy); Telescope; Active galactic nucleus; Millimeter; Radio galaxy; Redshift; Optics","score_opus":0.04883612750137268,"score_gpt":0.2724534527573494,"score_spread":0.22361732525597672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150780877","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3984403,0.0017074867,0.0020622814,0.00038166018,0.000098991004,0.00015826005,0.58533794,0.0008189372,0.010994114],"genre_scores_gemma":[0.27258614,0.0019971798,0.0023968464,0.00011024578,0.00020536508,0.00018721366,0.71666723,0.00020934526,0.0056404355],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989598,0.00007336449,0.00013639596,0.0001424544,0.0005733274,0.00011478365],"domain_scores_gemma":[0.9947482,0.0007860685,0.0017072662,0.00062807323,0.0016711532,0.00045922253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008479515,0.0002990607,0.0006313442,0.008270432,0.0002923395,0.0006142427,0.00061242795,0.00035364318,0.006710411],"category_scores_gemma":[0.003527548,0.00029956608,0.00029152623,0.012544082,0.00020191235,0.0006616306,0.0010192688,0.0004575697,0.007101907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026187982,0.00010864813,0.7752509,0.00021510296,0.00016665075,0.0001029278,0.00023456245,0.0009722094,0.0014892652,0.0005537802,0.1732488,0.047395192],"study_design_scores_gemma":[0.000026384567,0.000020222727,0.9840375,0.000014101377,0.000029493907,0.00011431297,0.00010042786,0.00027715383,0.00019126557,0.00006208939,0.015119412,0.000007660208],"about_ca_topic_score_codex":0.018532686,"about_ca_topic_score_gemma":0.020008255,"teacher_disagreement_score":0.018532686,"about_ca_system_score_codex":0.00040954835,"about_ca_system_score_gemma":0.00077904266,"threshold_uncertainty_score":0.036849618},"labels":[],"label_agreement":null},{"id":"W2150920983","doi":"10.1088/0004-637x/762/2/92","title":"RAPID TeV GAMMA-RAY FLARING OF BL LACERTAE","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Flare; Blazar; Astrophysics; Crab Nebula; Gamma ray; Superluminal motion; Light curve; Astronomy; BL Lac object; Flux (metallurgy); Fermi Gamma-ray Space Telescope; Photon; Optics","score_opus":0.011506956719785816,"score_gpt":0.2212876092539651,"score_spread":0.20978065253417927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150920983","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966126,0.0011006532,0.00038321537,0.00006632883,0.000012596684,0.000015213742,0.00035759495,0.00009784459,0.0013539711],"genre_scores_gemma":[0.99817216,0.00022241905,0.00044359855,0.00007376234,0.000033259977,0.000004813809,0.0006467402,0.000011715904,0.00039147737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997998,0.000011150842,0.000010011157,0.00005866744,0.000065865905,0.000054505377],"domain_scores_gemma":[0.9995753,0.000031772535,0.00020742691,0.00003851743,0.00005836367,0.00008852502],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017332601,0.00036733452,0.00040253645,0.001096319,0.00043155457,0.000884788,0.00036795138,0.0006451037,0.00093593047],"category_scores_gemma":[0.0005804661,0.00018821027,0.00033721232,0.0005581678,0.00030524153,0.00032961587,0.0006377696,0.00049691804,0.0003477613],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005178045,0.000106282394,0.6360786,0.00016132853,0.00022696986,0.0076540853,0.0010801707,0.00037029065,0.3142387,0.00021278516,0.0011584226,0.038194668],"study_design_scores_gemma":[0.000007891791,0.00015260204,0.98520446,0.000010697611,0.000035464545,0.004410247,0.0001200304,0.0002140949,0.0072135134,0.000078706675,0.002535834,0.0000164369],"about_ca_topic_score_codex":0.0029193733,"about_ca_topic_score_gemma":0.004818996,"teacher_disagreement_score":0.0029193733,"about_ca_system_score_codex":0.0004597507,"about_ca_system_score_gemma":0.00009265356,"threshold_uncertainty_score":0.005804777},"labels":[],"label_agreement":null},{"id":"W2150932047","doi":"10.1088/0004-637x/814/2/110","title":"Bicep2. III. INSTRUMENTAL SYSTEMATICS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"","keywords":"Spurious relationship; Physics; Systematics; Computational physics; Optics; Statistics; Mathematics","score_opus":0.01877466446082714,"score_gpt":0.2327473905823312,"score_spread":0.21397272612150406,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150932047","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.485533,0.0005981804,0.30928698,0.0016371734,0.0004740296,0.0006039464,0.08667958,0.03596042,0.07922665],"genre_scores_gemma":[0.733303,0.00018470059,0.19150318,0.0009086358,0.00008948955,0.0011393662,0.057769656,0.0080453195,0.0070567303],"study_design_codex":"simulation_or_modeling","study_design_gemma":"not_applicable","domain_scores_codex":[0.9983198,0.0006333816,0.000053040127,0.00030536432,0.0004972695,0.00019108846],"domain_scores_gemma":[0.99491125,0.001888493,0.00038207808,0.0014106184,0.001254898,0.00015274613],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0056399535,0.00090643874,0.0005883163,0.0009154838,0.0011243969,0.0011681992,0.0022701297,0.0008084109,0.008956212],"category_scores_gemma":[0.011010585,0.00079259,0.001165112,0.0017786192,0.0005451257,0.0012093788,0.0012909177,0.0012788202,0.0019506819],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013722983,0.0002927469,0.1362603,0.0006657131,0.0009856878,0.0006156652,0.0005568573,0.60311013,0.010105194,0.072643064,0.11087307,0.06251924],"study_design_scores_gemma":[0.0003658762,0.00023754721,0.036394574,0.00008142559,0.0001503149,0.00043176915,0.00008999901,0.86920637,0.018127725,0.025699152,0.049059846,0.00015549426],"about_ca_topic_score_codex":0.014946454,"about_ca_topic_score_gemma":0.012820815,"teacher_disagreement_score":0.014946454,"about_ca_system_score_codex":0.0009853297,"about_ca_system_score_gemma":0.0015468826,"threshold_uncertainty_score":0.029961526},"labels":[],"label_agreement":null},{"id":"W2150988709","doi":"10.1088/0004-637x/784/2/169","title":"RADIATION MAGNETOHYDRODYNAMIC SIMULATIONS OF THE FORMATION OF HOT ACCRETION DISK CORONAE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Corona (planetary geology); Photosphere; Magnetohydrodynamics; Accretion (finance); Radiative cooling; Dissipation; Coronal radiative losses; Radiative transfer; Intermediate polar; Magnetohydrodynamic turbulence; Active galactic nucleus; Magnetic field; Astronomy; Spectral line; Solar wind; Thermodynamics; Optics; Galaxy; Stars; Coronal mass ejection","score_opus":0.007261449225843426,"score_gpt":0.21679602885876742,"score_spread":0.209534579632924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150988709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99113387,0.00015755338,0.0019712467,0.00032686317,0.00003264898,0.000033554872,0.0005454751,0.00013810064,0.005660666],"genre_scores_gemma":[0.9970784,0.00005929726,0.0017049857,0.000086357024,0.000012056291,0.00003370273,0.0004064883,0.000036267018,0.00058249425],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998691,0.000037048147,0.0000071640857,0.000020232059,0.000022021484,0.0000443437],"domain_scores_gemma":[0.99903345,0.00053840014,0.0001025693,0.000043202504,0.000099617624,0.00018285913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033959176,0.0004574378,0.0005707537,0.00040549488,0.0005700682,0.00080782874,0.0010218803,0.0011379264,0.0016796476],"category_scores_gemma":[0.0018746636,0.0003567939,0.0006380387,0.00053895795,0.0006838132,0.00044739456,0.00068358704,0.00097047846,0.00014270564],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030010604,0.00018558651,0.011546167,0.000048109552,0.00009896692,0.00026463484,0.00014030465,0.9805893,0.002566829,0.0020193006,0.00069670746,0.0015440158],"study_design_scores_gemma":[0.00008056639,0.000045136276,0.0027945365,0.0000048581724,0.00001040794,0.000015536503,0.000044118628,0.995992,0.0002681242,0.0004802686,0.0002562317,0.000008226263],"about_ca_topic_score_codex":0.015570026,"about_ca_topic_score_gemma":0.008024468,"teacher_disagreement_score":0.015570026,"about_ca_system_score_codex":0.0010679002,"about_ca_system_score_gemma":0.0006062568,"threshold_uncertainty_score":0.030958772},"labels":[],"label_agreement":null},{"id":"W2150995848","doi":"10.1086/521818","title":"Multiwavelength Study of Massive Galaxies at<i>z</i>∼2. I. Star Formation and Galaxy Growth","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1603,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Luminous infrared galaxy; Galaxy; Star formation; Astronomy; Photometry (optics); Galaxy formation and evolution; Galaxy merger; Elliptical galaxy; Peculiar galaxy; Stellar mass; Redshift; Radio galaxy; Lenticular galaxy; Stars","score_opus":0.007861752395955128,"score_gpt":0.2153524911587156,"score_spread":0.20749073876276047,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2150995848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978492,0.0002688266,0.00013254823,0.000041851996,0.0000021242788,0.0000026145226,0.00034896328,0.000011020408,0.0013428609],"genre_scores_gemma":[0.9983108,0.0001219859,0.00031824672,0.00001741557,0.0000075115177,0.0000037106454,0.0003857887,0.000007199478,0.0008273962],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995995,0.0000048239717,0.0000022913089,0.000012342997,0.000005660097,0.000015023267],"domain_scores_gemma":[0.9997204,0.000046256555,0.0000829489,0.000033472512,0.000028793505,0.0000880384],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012237571,0.00012896444,0.0001324671,0.0009037627,0.00025073576,0.00033646586,0.00017082505,0.00014155328,0.0016593933],"category_scores_gemma":[0.00023311297,0.00016513724,0.00020277049,0.0007165314,0.0001416571,0.0002530847,0.0003289814,0.00024718975,0.0003351114],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048639692,0.00015312035,0.8458675,0.00006748346,0.00009437529,0.0005591354,0.00040199317,0.0006840531,0.13271472,0.0008647645,0.00091408717,0.017192354],"study_design_scores_gemma":[0.0000018779418,0.00001767043,0.99861443,0.00000177351,0.0000060734874,0.00015430787,0.000046284196,0.00014726409,0.0006942401,0.000068283356,0.00024616084,0.0000015439324],"about_ca_topic_score_codex":0.004066382,"about_ca_topic_score_gemma":0.00850718,"teacher_disagreement_score":0.004066382,"about_ca_system_score_codex":0.0003006989,"about_ca_system_score_gemma":0.000087929584,"threshold_uncertainty_score":0.00808543},"labels":[],"label_agreement":null},{"id":"W2151165291","doi":"10.1088/0004-637x/750/2/105","title":"LARGE-AMPLITUDE VARIATIONS OF AN L/T TRANSITION BROWN DWARF: MULTI-WAVELENGTH OBSERVATIONS OF PATCHY, HIGH-CONTRAST CLOUD FEATURES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":208,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec à Montréal; University of Toronto","funders":"","keywords":"Opacity; Brown dwarf; Molecular cloud; Amplitude; Cloud computing; Cloud physics; Infrared","score_opus":0.019694527170711046,"score_gpt":0.2514427600355467,"score_spread":0.23174823286483567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2151165291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993461,0.00003089532,0.00007123324,0.000013633221,0.0000021027797,0.0000023730965,0.00013026,0.000018875488,0.00038456212],"genre_scores_gemma":[0.9995912,0.000014909685,0.00014341793,0.000010036138,0.0000063191337,0.000002736682,0.00015337317,0.0000029994721,0.000075022144],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995255,0.0000027867725,0.0000020629566,0.00001842079,0.000010853091,0.000013371202],"domain_scores_gemma":[0.99987483,0.0000088993165,0.000040523224,0.000011786599,0.000009921251,0.000054023567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008116461,0.00019711847,0.00018184223,0.0004980001,0.00030939048,0.00025431687,0.00023709101,0.00028187572,0.00044956434],"category_scores_gemma":[0.00017778581,0.0001226015,0.00016014569,0.00035112517,0.00013929165,0.0001661246,0.0002936146,0.00020089648,0.0001438272],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053481426,0.00017948047,0.48306862,0.000059150316,0.00009610535,0.0016933249,0.00041104257,0.0013517303,0.5014162,0.00027247836,0.0009660639,0.009950995],"study_design_scores_gemma":[0.000013202301,0.000056410372,0.99304295,0.0000032555804,0.000014335801,0.00036415143,0.000065936765,0.00134415,0.0046028206,0.00004688646,0.00043922703,0.0000067396554],"about_ca_topic_score_codex":0.00292788,"about_ca_topic_score_gemma":0.005743288,"teacher_disagreement_score":0.00292788,"about_ca_system_score_codex":0.00023885396,"about_ca_system_score_gemma":0.000073400355,"threshold_uncertainty_score":0.0058216453},"labels":[],"label_agreement":null},{"id":"W2151969967","doi":"10.1088/0004-637x/691/1/425","title":"RAPIDLY SPINNING BLACK HOLES IN QUASARS: AN OPEN QUESTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Astrophysics; Physics; Supermassive black hole; Redshift; Accretion (finance); Radiative transfer; Radiation pressure; Astronomy; Galaxy; Quantum mechanics","score_opus":0.013130094709260607,"score_gpt":0.26458350848963597,"score_spread":0.25145341378037533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2151969967","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.43571144,0.3026494,0.0148635255,0.2141406,0.0018520126,0.00005349471,0.0007134747,0.00022218734,0.029793788],"genre_scores_gemma":[0.8950496,0.07887063,0.0047163004,0.008158892,0.0091357175,0.000038295373,0.00033421497,0.00004335368,0.0036528967],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9993799,0.00016434393,0.000034731456,0.00017621377,0.00007559442,0.0001691252],"domain_scores_gemma":[0.99214256,0.0038565686,0.0018399458,0.0006792456,0.0006421879,0.0008394133],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0047494806,0.0005267353,0.001260086,0.0012048038,0.001220729,0.0034073764,0.0020354309,0.0049975305,0.006486118],"category_scores_gemma":[0.008698609,0.0004265021,0.0005862944,0.0013185763,0.0057826284,0.014797658,0.0018797016,0.0022509282,0.001434883],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003289809,0.00052600435,0.16870987,0.0018814644,0.0004491373,0.0012601737,0.002289042,0.0028270422,0.0038379983,0.31201935,0.028666992,0.4772039],"study_design_scores_gemma":[0.00008801809,0.00025926266,0.18077907,0.0008707195,0.00008869549,0.0034196104,0.004660142,0.0037129573,0.00086328224,0.757109,0.048006583,0.0001425766],"about_ca_topic_score_codex":0.0022105817,"about_ca_topic_score_gemma":0.001403312,"teacher_disagreement_score":0.006486118,"about_ca_system_score_codex":0.00080391124,"about_ca_system_score_gemma":0.00078534934,"threshold_uncertainty_score":0.025117934},"labels":[],"label_agreement":null},{"id":"W2152064438","doi":"10.1088/0004-637x/693/2/1449","title":"GROWTH OF MAGNETIC FIELDS INDUCED BY TURBULENT MOTIONS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Magnetohydrodynamics; Magnetic field; Magnetohydrodynamic turbulence; Turbulence; Magnetic energy; Magnetic pressure; Isotropy; Magnetohydrodynamic drive; Kinetic energy; Field (mathematics); Computational physics; Classical mechanics; Mechanics; Magnetization; Quantum mechanics","score_opus":0.006088169175937466,"score_gpt":0.21486897525533624,"score_spread":0.20878080607939878,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152064438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929283,0.00007179593,0.0028159348,0.00017862738,0.00003328704,0.000022514376,0.000191235,0.000107601285,0.0036507084],"genre_scores_gemma":[0.9983181,0.000038650425,0.0011039296,0.000019827818,0.000007998636,0.00001796041,0.00015111126,0.000016125869,0.00032634058],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998617,0.000029389343,0.000010392726,0.000018906761,0.000027805056,0.00005188213],"domain_scores_gemma":[0.9994198,0.00022249816,0.00010734894,0.000041386545,0.00007069261,0.00013834222],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002343786,0.00041561064,0.00041216586,0.00043430686,0.00060790643,0.00092049513,0.0006346445,0.00064872927,0.0012889071],"category_scores_gemma":[0.002025767,0.00023279712,0.0003953514,0.000463628,0.0010046341,0.00055591104,0.00075718795,0.00072089676,0.00009956439],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041365056,0.00021907054,0.012120643,0.0000820406,0.000057908917,0.00033628015,0.00018900396,0.9610418,0.015686942,0.0065194797,0.00053101935,0.002802118],"study_design_scores_gemma":[0.00007830896,0.00007315575,0.003246389,0.000009113375,0.000012874772,0.000024162127,0.00004143178,0.99283594,0.00268881,0.00069110224,0.0002825471,0.000016244068],"about_ca_topic_score_codex":0.01061084,"about_ca_topic_score_gemma":0.0043643084,"teacher_disagreement_score":0.01061084,"about_ca_system_score_codex":0.0008469276,"about_ca_system_score_gemma":0.0007589098,"threshold_uncertainty_score":0.021098197},"labels":[],"label_agreement":null},{"id":"W2152309824","doi":"10.1086/522336","title":"The Molecular Gas Environment around Two Herbig Ae/Be Stars: Resolving the Outflows of LkHα 198 and LkHα 225S","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Stars; Outflow; Astrophysics; Molecular cloud; Line (geometry); Astronomy; Meteorology","score_opus":0.00878871266746322,"score_gpt":0.23443196135522948,"score_spread":0.22564324868776625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152309824","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99888426,0.00003983918,0.0001768228,0.000018550134,0.0000013207457,0.0000040933232,0.00005901701,0.000013820883,0.00080218015],"genre_scores_gemma":[0.9988135,0.000029266701,0.0006660836,0.000031276028,0.000005163259,0.0000042352412,0.00025625646,0.000005435119,0.00018880251],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999386,0.0000038783096,0.0000023678303,0.000020781234,0.000015450283,0.000018836186],"domain_scores_gemma":[0.99987984,0.00001016212,0.000030457984,0.000007592626,0.0000148488925,0.000056956214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010814141,0.00017477132,0.00019796475,0.0005927995,0.0004688013,0.00038072368,0.00022088838,0.00023210628,0.00064325664],"category_scores_gemma":[0.00017400477,0.00016761934,0.00009385708,0.00028073293,0.00017587029,0.00020487283,0.00042681512,0.00027464077,0.0001734472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050400215,0.00013294621,0.6683695,0.00003375142,0.000053724038,0.0006183452,0.00037578805,0.0006361351,0.31618896,0.00023586921,0.0003244402,0.012526582],"study_design_scores_gemma":[0.000020989737,0.000036986406,0.99397177,0.0000044664243,0.000012251556,0.00011641203,0.000148183,0.0010846194,0.003858899,0.0000554475,0.0006863134,0.0000035221174],"about_ca_topic_score_codex":0.004773528,"about_ca_topic_score_gemma":0.012522882,"teacher_disagreement_score":0.004773528,"about_ca_system_score_codex":0.0003259957,"about_ca_system_score_gemma":0.00013285241,"threshold_uncertainty_score":0.009491503},"labels":[],"label_agreement":null},{"id":"W2152317214","doi":"10.1088/0004-637x/747/2/108","title":"ASTEROSEISMOLOGY OF THE NEARBY SN-II PROGENITOR: RIGEL. I. THE<i>MOST</i>HIGH-PRECISION PHOTOMETRY AND RADIAL VELOCITY MONITORING","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Radial velocity; Photometry (optics); Supergiant; Asteroseismology; Supernova; Flux (metallurgy)","score_opus":0.011599052369310971,"score_gpt":0.23874037595262,"score_spread":0.22714132358330902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152317214","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99775946,0.00014174663,0.00014234376,0.00001438035,0.0000016231985,0.0000049812043,0.00031290477,0.000010978885,0.0016115953],"genre_scores_gemma":[0.9989813,0.000037459613,0.00019506458,0.000007642858,0.00000250321,0.0000016985737,0.0004800298,0.000002658485,0.0002916135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999515,0.000007044999,0.0000033476208,0.000018682147,0.0000093412555,0.0000102051945],"domain_scores_gemma":[0.9997744,0.000018243793,0.00010496646,0.00002765085,0.000025427189,0.000049351675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001667348,0.00012708362,0.00009782812,0.00061883195,0.00019305608,0.00031201582,0.00018378721,0.00019659405,0.0005351374],"category_scores_gemma":[0.0002999613,0.000054515822,0.00010134087,0.0002475709,0.00018203948,0.00019572153,0.00034279653,0.00016006737,0.00023456439],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028735524,0.000054075215,0.92508143,0.000023200038,0.000025760706,0.0013558182,0.00025442976,0.00055224745,0.061554555,0.00031202324,0.00027976494,0.010219308],"study_design_scores_gemma":[0.0000017389942,0.000059619208,0.9956091,0.0000029220657,0.000006152894,0.0010825929,0.000060816372,0.0004439452,0.0018907568,0.000059800288,0.0007787495,0.000003953962],"about_ca_topic_score_codex":0.0022546216,"about_ca_topic_score_gemma":0.004498,"teacher_disagreement_score":0.0022546216,"about_ca_system_score_codex":0.00019632935,"about_ca_system_score_gemma":0.00007839556,"threshold_uncertainty_score":0.0044829845},"labels":[],"label_agreement":null},{"id":"W2152356720","doi":"10.1088/0004-637x/697/1/807","title":"GRAIN ALIGNMENT IN OMC1 AS DEDUCED FROM OBSERVED LARGE CIRCULAR POLARIZATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Circular polarization; Polarization (electrochemistry); Axial ratio; Optics; Scattering; Dimensionless quantity; Wavelength; Multipole expansion; Molecular physics; Chemistry; Quantum mechanics","score_opus":0.013731283152886133,"score_gpt":0.24021788790497092,"score_spread":0.2264866047520848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152356720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99620783,0.00013779548,0.0007430879,0.00003255441,0.0000050285716,0.0000087707285,0.00029366638,0.00003454892,0.0025367779],"genre_scores_gemma":[0.99732995,0.00006195904,0.0013055729,0.000029334586,0.00000365855,0.000009753064,0.0009156688,0.000022898977,0.00032108926],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99968326,0.000007489769,0.000007604734,0.00008990161,0.00010301552,0.00010874082],"domain_scores_gemma":[0.99948716,0.000084262254,0.00013389405,0.000043593827,0.00016069539,0.00009028984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000284336,0.00038857159,0.00047103362,0.0013054053,0.0013250444,0.0009827609,0.0006465427,0.0006742435,0.00085561525],"category_scores_gemma":[0.00077008986,0.00038818727,0.00017387557,0.001697004,0.0006596649,0.00043676153,0.000696613,0.0005697881,0.00020163416],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008336924,0.00016006571,0.2619413,0.0002807232,0.000049503218,0.0016801889,0.0009754736,0.0116936555,0.69466853,0.0037004577,0.0017350172,0.02228135],"study_design_scores_gemma":[0.000046352838,0.000082063656,0.8276001,0.00004677032,0.000035033765,0.0005275945,0.0008494537,0.0456237,0.11966676,0.0009897625,0.004461939,0.00007048598],"about_ca_topic_score_codex":0.03173189,"about_ca_topic_score_gemma":0.025180392,"teacher_disagreement_score":0.03173189,"about_ca_system_score_codex":0.0026101477,"about_ca_system_score_gemma":0.00056762615,"threshold_uncertainty_score":0.06309438},"labels":[],"label_agreement":null},{"id":"W2152498713","doi":"10.1086/376754","title":"The Tully‐Fisher Relation of Barred Galaxies","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Tully–Fisher relation; Galaxy; Luminous infrared galaxy; Surface brightness; Astronomy; Peculiar galaxy; Disc; Fundamental plane (elliptical galaxies); Disc galaxy; Galaxy rotation curve; Elliptical galaxy; Galaxy formation and evolution","score_opus":0.00628511432666526,"score_gpt":0.1985024308775107,"score_spread":0.19221731655084545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152498713","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98148715,0.00085871783,0.009715308,0.00012380574,0.000007822973,0.000008378254,0.00024315352,0.00005816671,0.0074974853],"genre_scores_gemma":[0.9980573,0.00016778497,0.0012835121,0.000022262273,0.000014235265,0.0000053239123,0.0001987696,0.0000056616677,0.00024505245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995999,0.00006275304,0.000024632303,0.0001321082,0.000109716304,0.000070905015],"domain_scores_gemma":[0.99405164,0.0023666497,0.0017018196,0.0008611528,0.0004670238,0.00055181567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008702841,0.00016772102,0.0002450903,0.0019409069,0.00057231553,0.0010353181,0.0003175203,0.00027808902,0.0021879715],"category_scores_gemma":[0.008534423,0.00015200824,0.00017312418,0.0008666822,0.0011628828,0.0015688728,0.00072766026,0.0005664358,0.00025446943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015161882,0.000056170273,0.875833,0.000057216384,0.00006744979,0.00015200132,0.0024821332,0.0030523455,0.008399957,0.055385277,0.0011284909,0.05323428],"study_design_scores_gemma":[0.000011534926,0.000072009316,0.9231679,0.000028968365,0.000019716032,0.00039572545,0.00035869784,0.008696875,0.0012569978,0.061189637,0.0047644917,0.000037468482],"about_ca_topic_score_codex":0.0037639241,"about_ca_topic_score_gemma":0.002479841,"teacher_disagreement_score":0.0037639241,"about_ca_system_score_codex":0.0006040685,"about_ca_system_score_gemma":0.00015725022,"threshold_uncertainty_score":0.007484019},"labels":[],"label_agreement":null},{"id":"W2152540352","doi":"10.1088/0004-637x/694/2/1200","title":"HIGH-RESOLUTION CMB POWER SPECTRUM FROM THE COMPLETE ACBAR DATA SET","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":320,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Cosmic microwave background; Bolometer; Cosmology; Spectral density; Anisotropy; Cosmic background radiation; Sky; Detector; Planck","score_opus":0.019518079470384826,"score_gpt":0.25945561460315675,"score_spread":0.2399375351327719,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152540352","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8705438,0.0006367964,0.013132738,0.00022039303,0.000098459604,0.00008952308,0.10088463,0.0031008709,0.0112927025],"genre_scores_gemma":[0.76226664,0.00025353502,0.018048655,0.00010569748,0.0001526984,0.00014389039,0.21700187,0.00060293946,0.0014240639],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99922,0.00011331059,0.000037027767,0.00020568266,0.00031647302,0.000107413085],"domain_scores_gemma":[0.99853516,0.00022329985,0.00026183145,0.000442418,0.0003688811,0.00016835766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009430817,0.00094344123,0.0005330703,0.0029304035,0.00031758597,0.0010418762,0.0007244829,0.00037628796,0.004763826],"category_scores_gemma":[0.0018818473,0.00034415888,0.0008580446,0.0030621807,0.00016040228,0.00062961935,0.00091089535,0.00063237915,0.0024662567],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014789802,0.00047608415,0.6325455,0.00088184926,0.0016705967,0.0013900883,0.0006343912,0.05014506,0.054299284,0.0037441277,0.0655985,0.18713556],"study_design_scores_gemma":[0.000113696726,0.00007984975,0.9123792,0.000042329895,0.00015146578,0.00041673376,0.00014105567,0.02871647,0.00884862,0.0014288813,0.04759879,0.0000828893],"about_ca_topic_score_codex":0.0064412816,"about_ca_topic_score_gemma":0.007217789,"teacher_disagreement_score":0.0064412816,"about_ca_system_score_codex":0.00038592378,"about_ca_system_score_gemma":0.00025770353,"threshold_uncertainty_score":0.015936553},"labels":[],"label_agreement":null},{"id":"W2152540448","doi":"10.1088/0004-637x/794/1/10","title":"NON-AXISYMMETRIC FLOWS ON HOT JUPITERS WITH OBLIQUE MAGNETIC FIELDS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Hot Jupiter; Magnetic field; Planet; Magnetic dipole; Advection; Mercury's magnetic field; Dipole; Magnetohydrodynamics; L-shell","score_opus":0.003462686368393487,"score_gpt":0.19257431937205374,"score_spread":0.18911163300366027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152540448","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9862217,0.00013461613,0.009586933,0.00013067579,0.000023515642,0.00002130219,0.000057835154,0.00006538512,0.0037579935],"genre_scores_gemma":[0.9968924,0.00010913962,0.001848133,0.000020419844,0.00003381697,0.00001053066,0.000055082288,0.000019007088,0.0010114146],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994254,0.000018069415,0.0000029016885,0.000012719728,0.000009735149,0.000013978671],"domain_scores_gemma":[0.99974877,0.000046439625,0.00011553317,0.000017101169,0.000024003553,0.0000482694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013284126,0.000409441,0.0003004777,0.00048382254,0.00043323563,0.00067433895,0.0003270454,0.00038323936,0.0009376362],"category_scores_gemma":[0.00087830983,0.00019527695,0.00038792574,0.00021108784,0.00085826614,0.00043393686,0.0005155172,0.00024712423,0.00008107774],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059119647,0.0002959195,0.048200157,0.000141284,0.00016748138,0.0044495966,0.0010385093,0.6688892,0.13366725,0.1232155,0.0019193147,0.017424675],"study_design_scores_gemma":[0.000070741204,0.00008466291,0.021266278,0.000008536311,0.000018635914,0.00021796601,0.00012699545,0.9632961,0.002531087,0.011720935,0.0006324004,0.000025668653],"about_ca_topic_score_codex":0.0056767,"about_ca_topic_score_gemma":0.0030024156,"teacher_disagreement_score":0.0056767,"about_ca_system_score_codex":0.0007599319,"about_ca_system_score_gemma":0.00033300024,"threshold_uncertainty_score":0.011287272},"labels":[],"label_agreement":null},{"id":"W2152668089","doi":"10.1088/0004-637x/695/1/101","title":"RED NUGGETS AT<i>z</i>∼ 1.5: COMPACT PASSIVE GALAXIES AND THE FORMATION OF THE KORMENDY RELATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":342,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Galaxy; Physics; Galaxy formation and evolution; Stellar mass; Luminosity; Stars; Astronomy; Universe; Effective radius; Luminous infrared galaxy; Star formation","score_opus":0.005752058303105995,"score_gpt":0.20035374193219846,"score_spread":0.19460168362909247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152668089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99847776,0.00022964424,0.00018180895,0.000024503493,0.0000013017473,0.0000022323122,0.000068185516,0.0000145104195,0.0010000272],"genre_scores_gemma":[0.9995908,0.000050740142,0.00015952207,0.000008086671,0.0000028813874,0.0000015284526,0.00008592228,0.0000020723,0.00009837087],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985623,0.00001547238,0.000007859804,0.00004114969,0.000029757342,0.000049440278],"domain_scores_gemma":[0.9994049,0.000085081185,0.00029859884,0.0000653487,0.000027376873,0.00011872005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032578598,0.00024517468,0.00029255418,0.001372825,0.00046094344,0.00090755575,0.00041191935,0.00024322589,0.0007522768],"category_scores_gemma":[0.0008552901,0.00018215927,0.000107847394,0.0009665512,0.0008084414,0.0006532955,0.00086205645,0.00026206713,0.00018964236],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019741371,0.000032986452,0.97514355,0.000029848507,0.000021532805,0.00040863917,0.0012710647,0.00035926516,0.008323402,0.0018349725,0.00030082682,0.01207649],"study_design_scores_gemma":[0.0000043728924,0.00002449804,0.9963515,0.000008287536,0.000010790128,0.00042956238,0.00032365503,0.0005892016,0.0008541329,0.00052867364,0.00086870533,0.0000065553495],"about_ca_topic_score_codex":0.0028404521,"about_ca_topic_score_gemma":0.0045105782,"teacher_disagreement_score":0.0028404521,"about_ca_system_score_codex":0.00039282627,"about_ca_system_score_gemma":0.00010868839,"threshold_uncertainty_score":0.005647838},"labels":[],"label_agreement":null},{"id":"W2152678599","doi":"10.1088/0004-637x/789/1/52","title":"THE X-RAY LUMINOSITY FUNCTIONS OF FIELD LOW-MASS X-RAY BINARIES IN EARLY-TYPE GALAXIES: EVIDENCE FOR A STELLAR AGE DEPENDENCE","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Natural Sciences and Engineering Research Council of Canada; Science and Technology Facilities Council; Space Telescope Science Institute; Northwestern University; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Globular cluster; Galaxy; Astronomy; Stellar population; Stellar mass; Luminosity; Hubble Deep Field; Population; Hubble space telescope; Star formation","score_opus":0.015250076114413348,"score_gpt":0.23764740411053287,"score_spread":0.22239732799611953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152678599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99823004,0.00012667362,0.00011029804,0.000035644578,0.0000014237382,0.0000018888484,0.00020107187,0.000010565648,0.0012823388],"genre_scores_gemma":[0.99909127,0.000035127163,0.000044537002,0.00001393185,0.0000024676526,0.0000013228158,0.00024114024,0.000004449915,0.0005657624],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999889,0.000018055323,0.000008244207,0.000035484696,0.000018138111,0.00003106291],"domain_scores_gemma":[0.9983292,0.00046301482,0.00043541347,0.00013923873,0.00019528446,0.00043778264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041016898,0.00012641586,0.00017153916,0.0013316694,0.0002642333,0.00089308823,0.0002555633,0.0003495369,0.0058983117],"category_scores_gemma":[0.0017787428,0.00016087989,0.00012497864,0.0006661853,0.00034178948,0.00062029075,0.000681187,0.0002709342,0.0011086199],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021474941,0.00004244767,0.99129057,0.000007846364,0.000013869884,0.000022594542,0.00018679097,0.00007496158,0.0026784374,0.00021609443,0.0001446257,0.005107054],"study_design_scores_gemma":[0.000001385958,0.000008915874,0.999564,0.0000012942497,0.000002033798,0.000026844025,0.000051726587,0.00011672006,0.00008986141,0.00005878733,0.00007748806,9.298593e-7],"about_ca_topic_score_codex":0.0071497927,"about_ca_topic_score_gemma":0.008655484,"teacher_disagreement_score":0.0071497927,"about_ca_system_score_codex":0.0003347292,"about_ca_system_score_gemma":0.00013230616,"threshold_uncertainty_score":0.01973188},"labels":[],"label_agreement":null},{"id":"W2152756270","doi":"10.1088/0004-637x/694/2/1147","title":"A<i>SPITZER</i>STUDY OF 21 AND 30 μm EMISSION IN SEVERAL GALACTIC CARBON-RICH PROTOPLANETARY NEBULAE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Astrophysics; Planetary nebula; Physics; Spitzer Space Telescope; Spectral line; Infrared; Astronomy; Emission spectrum; Absorption (acoustics); Spectroscopy; Telescope; Stars; Optics","score_opus":0.007518375603970344,"score_gpt":0.23101337011114778,"score_spread":0.22349499450717744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152756270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99911386,0.00017450994,0.00020311285,0.000011195022,0.0000011261192,0.0000026695448,0.000031514603,0.000008145446,0.00045393666],"genre_scores_gemma":[0.9981906,0.00014566863,0.00092964544,0.00002891864,0.000008390504,0.0000053725917,0.0003156231,0.000005928637,0.00036982304],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998982,0.000007830118,0.0000044772587,0.000031123327,0.000033842327,0.00002451655],"domain_scores_gemma":[0.9998323,0.00001906405,0.000057648434,0.000012599521,0.000035637364,0.000042723947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022564104,0.00028923614,0.00017563468,0.00091546285,0.0005021778,0.00039684615,0.0004026938,0.0002870051,0.00064797327],"category_scores_gemma":[0.00024748498,0.00017137142,0.00018735137,0.00039276652,0.00026927164,0.00026727098,0.0002822778,0.00024332912,0.00017516872],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002806666,0.00012252276,0.43184936,0.000072124196,0.00007675889,0.00079448905,0.00065468566,0.00052910455,0.5517344,0.00028891378,0.00018290777,0.013414166],"study_design_scores_gemma":[0.0000087925355,0.00017133736,0.973216,0.00000618306,0.00002053486,0.000815103,0.00015293044,0.0005310359,0.023755787,0.00007161153,0.001243687,0.000007060919],"about_ca_topic_score_codex":0.0018801839,"about_ca_topic_score_gemma":0.002181567,"teacher_disagreement_score":0.0018801839,"about_ca_system_score_codex":0.0003362327,"about_ca_system_score_gemma":0.000106743646,"threshold_uncertainty_score":0.003738463},"labels":[],"label_agreement":null},{"id":"W2152777658","doi":"10.1088/0004-637x/786/1/13","title":"CMB LENSING POWER SPECTRUM BIASES FROM GALAXIES AND CLUSTERS USING HIGH-ANGULAR RESOLUTION TEMPERATURE MAPS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cosmic microwave background; Galaxy; Weak gravitational lensing; Spectral density; Multipole expansion; Cosmic infrared background; Gravitational lens; Galaxy cluster; Cosmology","score_opus":0.008486259478571435,"score_gpt":0.20563044019561388,"score_spread":0.19714418071704246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152777658","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8467909,0.0004441985,0.14343537,0.00043018308,0.000040833005,0.000026397634,0.00032919517,0.00095487403,0.0075480253],"genre_scores_gemma":[0.9812557,0.00011197465,0.017835166,0.00004735842,0.000013099125,0.0000065662016,0.00024888216,0.00014429644,0.0003368771],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99947757,0.00016509442,0.00001979,0.00008823755,0.00019407774,0.00005520907],"domain_scores_gemma":[0.9969031,0.0018049729,0.00046899728,0.00043415983,0.00028806206,0.0001006734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015518315,0.00047083653,0.00026184958,0.0005945451,0.00027286573,0.0009929314,0.00059089,0.00036495854,0.001409306],"category_scores_gemma":[0.011154881,0.0003473953,0.0004481799,0.0007581598,0.0004325385,0.0009857692,0.0006568963,0.00046885852,0.00020999419],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007874003,0.0000837963,0.1918579,0.00029752348,0.00046659575,0.0003400139,0.00071405864,0.5962905,0.060703002,0.029120691,0.0020651433,0.117273316],"study_design_scores_gemma":[0.000048860413,0.00006375141,0.089244016,0.000068575726,0.00012675097,0.0002411268,0.000111419096,0.8595954,0.035566743,0.012818001,0.0020355275,0.000079788646],"about_ca_topic_score_codex":0.00926179,"about_ca_topic_score_gemma":0.007827864,"teacher_disagreement_score":0.00926179,"about_ca_system_score_codex":0.0008336489,"about_ca_system_score_gemma":0.00046934214,"threshold_uncertainty_score":0.01841575},"labels":[],"label_agreement":null},{"id":"W2152915695","doi":"10.1086/339323","title":"A<i>Far Ultraviolet Spectroscopic Explorer</i>Survey of Interstellar O<scp>vi</scp>Absorption in the Small Magellanic Cloud","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Milky Way; Galaxy; Metallicity; Small Magellanic Cloud; Line-of-sight; Interstellar medium; Astronomy; Stars; Galactic plane; Large Magellanic Cloud; Halo; Star formation","score_opus":0.02873769226398729,"score_gpt":0.23473346809468465,"score_spread":0.20599577583069736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2152915695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98664296,0.000289548,0.00047688637,0.000086598804,0.000007591871,0.000029992862,0.00956484,0.00011443466,0.0027871185],"genre_scores_gemma":[0.9669185,0.00028971207,0.0030546323,0.00013590374,0.000046895057,0.000039411458,0.027398422,0.000029915653,0.0020865896],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981624,0.000021278665,0.000009282645,0.000043113818,0.00006169412,0.000048363258],"domain_scores_gemma":[0.9990569,0.00005077319,0.00028682247,0.00006175282,0.00013297268,0.00041076564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002959379,0.00019321906,0.00017248865,0.0021480783,0.0003250786,0.0003060344,0.00024683835,0.00023346372,0.0014635705],"category_scores_gemma":[0.0003048553,0.000081438826,0.00020040214,0.0010608389,0.000110109206,0.00020707597,0.00038788727,0.00016833303,0.00045721047],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012777725,0.00013796896,0.9606469,0.000037274236,0.00011384834,0.00018589743,0.0001363413,0.00018731202,0.017315133,0.000089499095,0.003001838,0.018020079],"study_design_scores_gemma":[0.000006147942,0.000052152405,0.99665475,0.0000035765884,0.0000150434735,0.00010196368,0.000042523843,0.00012666178,0.0007581414,0.000015905356,0.0022204358,0.0000027452063],"about_ca_topic_score_codex":0.00892917,"about_ca_topic_score_gemma":0.018642303,"teacher_disagreement_score":0.00892917,"about_ca_system_score_codex":0.00021164127,"about_ca_system_score_gemma":0.0002533935,"threshold_uncertainty_score":0.017754376},"labels":[],"label_agreement":null},{"id":"W2153003086","doi":"10.1086/587736","title":"VERITAS Observations of the γ‐Ray Binary LS I +61 303","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":152,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Crab Nebula; Flux (metallurgy); Astrophysics; Orbital period; Photon; Energy spectrum; Gamma ray; Photon flux; Optics; Stars","score_opus":0.02842239137229464,"score_gpt":0.22880172214697406,"score_spread":0.20037933077467943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153003086","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99680567,0.000080455,0.00009880772,0.00003561073,0.0000050331632,0.000003928169,0.00046984004,0.000045132154,0.0024555332],"genre_scores_gemma":[0.99729055,0.000058834576,0.00046685725,0.000028501923,0.000008328029,0.0000052368864,0.0011856247,0.000015257958,0.00094071066],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987555,0.000008666128,0.0000053892104,0.00003201797,0.000049133636,0.000029225377],"domain_scores_gemma":[0.9996463,0.00004192557,0.00014927902,0.000037659258,0.00005267433,0.00007215516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022225524,0.00013947386,0.0002517716,0.0005770414,0.00046537342,0.000497529,0.0002989954,0.00031629152,0.0018225386],"category_scores_gemma":[0.00039290718,0.0002256843,0.00016787685,0.00051688333,0.00024920306,0.00024444947,0.0004902565,0.00039835737,0.0006353932],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020783795,0.00021012178,0.5607683,0.0001446979,0.0001353015,0.0017548004,0.0014201873,0.0019630338,0.39109236,0.0024947047,0.0063741505,0.031563926],"study_design_scores_gemma":[0.00009635588,0.0004376579,0.97876644,0.000028884828,0.00004437799,0.0011602113,0.00037249108,0.002712049,0.009521627,0.0002672122,0.0065667313,0.000025995045],"about_ca_topic_score_codex":0.0115132285,"about_ca_topic_score_gemma":0.027589215,"teacher_disagreement_score":0.0115132285,"about_ca_system_score_codex":0.0006091482,"about_ca_system_score_gemma":0.0003303281,"threshold_uncertainty_score":0.022892416},"labels":[],"label_agreement":null},{"id":"W2153016433","doi":"10.1088/0004-637x/790/1/6","title":"PARAMAGNETIC ALIGNMENT OF SMALL GRAINS: A NOVEL METHOD FOR MEASURING INTERSTELLAR MAGNETIC FIELDS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Paramagnetism; Polarization (electrochemistry); Magnetic field; Dipole; Wavelength; Interstellar medium; Magnetic moment","score_opus":0.023773136096622613,"score_gpt":0.25073387686568216,"score_spread":0.22696074076905953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153016433","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.41551885,0.000294518,0.57980716,0.0000832324,0.00007313584,0.0000820435,0.00029713463,0.0008429319,0.0030009993],"genre_scores_gemma":[0.8512664,0.00016229921,0.14727792,0.00003339735,0.000024340112,0.00007931239,0.00014600989,0.00007157471,0.00093882415],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998752,0.000012364736,0.000004478433,0.000051517916,0.000041432104,0.000014905816],"domain_scores_gemma":[0.999811,0.000042494103,0.00005841151,0.000032645992,0.00003278902,0.000022674114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013196381,0.00025074172,0.00021400403,0.0005441251,0.00020760323,0.00032892305,0.00056444306,0.0003198939,0.000672614],"category_scores_gemma":[0.00046172403,0.0002170236,0.00015209363,0.00041663687,0.00023839164,0.00047213063,0.0003390646,0.0005443118,0.00017593386],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016062288,0.00008169492,0.013179719,0.00008264223,0.000050876977,0.00013783225,0.00012823472,0.023021031,0.898365,0.0063087055,0.00034896226,0.058134753],"study_design_scores_gemma":[0.00005596836,0.00021154291,0.022825114,0.000010282926,0.00003965448,0.0002398664,0.00007809045,0.5270453,0.44067138,0.0043299263,0.0044284393,0.00006450402],"about_ca_topic_score_codex":0.0010738577,"about_ca_topic_score_gemma":0.0011384143,"teacher_disagreement_score":0.0010738577,"about_ca_system_score_codex":0.000329868,"about_ca_system_score_gemma":0.00021932472,"threshold_uncertainty_score":0},"labels":[],"label_agreement":null},{"id":"W2153050977","doi":"10.1088/0004-637x/763/2/93","title":"SPT-CL J0205–5829: A<i>z</i>= 1.32 EVOLVED MASSIVE GALAXY CLUSTER IN THE SOUTH POLE TELESCOPE SUNYAEV-ZEL'DOVICH EFFECT SURVEY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; California Institute of Technology; Massachusetts Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Physics; South Pole Telescope; Astrophysics; Sunyaev–Zel'dovich effect; Galaxy cluster; Astronomy; Redshift; Galaxy; Cosmology; Cluster (spacecraft); Stellar mass; Brightest cluster galaxy; Population; Star formation","score_opus":0.007458576998299925,"score_gpt":0.21181965102088654,"score_spread":0.2043610740225866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153050977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930005,0.0001493855,0.00008196797,0.00015704603,0.000015667496,0.00000862261,0.0035413273,0.000027970314,0.003017473],"genre_scores_gemma":[0.9927776,0.000067941495,0.00013722517,0.000059312548,0.0000145021,0.0000074195113,0.0053662155,0.000013020431,0.0015567024],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982363,0.000016106735,0.000007066882,0.00004872285,0.00004093043,0.000063629835],"domain_scores_gemma":[0.9996306,0.000015372341,0.00008871433,0.000028355777,0.000050831084,0.00018611012],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023427918,0.00010896745,0.00022017452,0.0009776922,0.00083649356,0.00055026094,0.00031561137,0.00021506051,0.0032921734],"category_scores_gemma":[0.0003670517,0.000098477954,0.00011733583,0.0009874903,0.00024345118,0.0002731221,0.0009160488,0.0002602477,0.0005903333],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015202121,0.00006364757,0.9802507,0.000024104847,0.000040669078,0.00025964505,0.00047014572,0.000077232595,0.0028032816,0.00061699987,0.00903847,0.006203137],"study_design_scores_gemma":[0.0000063288103,0.000008600067,0.99702495,0.000003840976,0.000008102751,0.000078846104,0.00026171582,0.00006858387,0.00008347042,0.000031318486,0.002422768,0.0000014833865],"about_ca_topic_score_codex":0.055144425,"about_ca_topic_score_gemma":0.112585925,"teacher_disagreement_score":0.055144425,"about_ca_system_score_codex":0.0003393597,"about_ca_system_score_gemma":0.0005321116,"threshold_uncertainty_score":0.10964692},"labels":[],"label_agreement":null},{"id":"W2153069790","doi":"10.1088/0004-637x/809/2/142","title":"THE SUPERLUMINOUS SN DES13S2cmm AS A SIGNATURE OF A QUARK-NOVA IN A HE-HMXB SYSTEM","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Neutron star; Astrophysics; Nova (rocket); Ejecta; Accretion (finance); Quark star; Black hole (networking); Strange matter; Supernova","score_opus":0.017840373425309128,"score_gpt":0.31543844894512646,"score_spread":0.2975980755198173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153069790","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99863297,0.000047939237,0.00012380948,0.000019469766,0.0000024786054,0.0000026216965,0.000077189994,0.000008944787,0.0010845775],"genre_scores_gemma":[0.9991548,0.000025963012,0.00025518588,0.000014626133,0.0000039061597,0.0000013523627,0.00022027285,0.0000036644683,0.00032019816],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999465,0.000006755475,0.0000025444942,0.000014714646,0.000014994881,0.000014547515],"domain_scores_gemma":[0.99982256,0.000020194491,0.00005934795,0.000018577653,0.000017119452,0.00006220976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001923762,0.0002846368,0.00017032622,0.00064860843,0.00028160147,0.00041575788,0.00018300764,0.00031131017,0.0011003405],"category_scores_gemma":[0.00023229225,0.00010772919,0.00018850138,0.0005024382,0.0002577689,0.00011336025,0.00034758067,0.00018605449,0.00019433357],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005724849,0.00006311099,0.9007102,0.000037617752,0.000054335957,0.0028298725,0.000177227,0.0012252957,0.08185988,0.0027022462,0.00066150754,0.009106024],"study_design_scores_gemma":[0.000022362015,0.00008207049,0.9868976,0.0000068639356,0.000016088148,0.0017608304,0.00010705071,0.0045170467,0.0040956954,0.000584554,0.0019027473,0.0000071737977],"about_ca_topic_score_codex":0.0050216354,"about_ca_topic_score_gemma":0.014511958,"teacher_disagreement_score":0.0050216354,"about_ca_system_score_codex":0.00040418544,"about_ca_system_score_gemma":0.00014921276,"threshold_uncertainty_score":0.009984791},"labels":[],"label_agreement":null},{"id":"W2153152528","doi":"10.1088/0004-637x/807/2/180","title":"STAR FORMATION AND THE INTERSTELLAR MEDIUM IN<i>z</i>&gt;6 UV-LUMINOUS LYMAN-BREAK GALAXIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Interstellar medium; Redshift; Star formation; Reionization; Luminous infrared galaxy; Line (geometry); Emission spectrum; Millimeter","score_opus":0.00949919915987208,"score_gpt":0.2046734525503277,"score_spread":0.19517425339045563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153152528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997557,0.000064575965,0.000009393154,0.000009516575,6.205486e-7,5.422441e-7,0.000029203848,0.0000016546667,0.00012878363],"genre_scores_gemma":[0.9998115,0.000039383634,0.000026732041,0.0000040071395,0.00000201931,5.3667833e-7,0.00006041165,5.9502116e-7,0.000054808443],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991345,0.000013975691,0.00000541056,0.000019293537,0.000014441457,0.000033442022],"domain_scores_gemma":[0.9994703,0.000050487673,0.00027247917,0.000016752467,0.000022429807,0.00016754313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020617542,0.00018135652,0.00016152223,0.0013677471,0.00036204158,0.00071398856,0.00024439004,0.0003233748,0.00075616327],"category_scores_gemma":[0.00048807412,0.00013629238,0.00012519777,0.00061747927,0.00043166403,0.00037015998,0.0005530197,0.00029184212,0.00018683313],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021110127,0.00006917531,0.98916477,0.0000085712845,0.000022227174,0.00016831905,0.00031334,0.000109275854,0.007227296,0.00013604283,0.00005327422,0.0025166343],"study_design_scores_gemma":[0.0000028044933,0.000028374343,0.9993955,0.0000013986494,0.000004213606,0.00008062704,0.00009604557,0.00007384915,0.00021171772,0.000038671293,0.00006549858,0.0000012435787],"about_ca_topic_score_codex":0.005119985,"about_ca_topic_score_gemma":0.007933035,"teacher_disagreement_score":0.005119985,"about_ca_system_score_codex":0.0003859177,"about_ca_system_score_gemma":0.00009919293,"threshold_uncertainty_score":0.010180354},"labels":[],"label_agreement":null},{"id":"W2153535686","doi":"10.1088/0004-637x/707/2/1836","title":"THE BLAST SURVEY OF THE VELA MOLECULAR CLOUD: PHYSICAL PROPERTIES OF THE DENSE CORES IN VELA-D","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"","keywords":"Vela; Physics; Astrophysics; Protostar; Molecular cloud; Young stellar object; Luminosity; Star formation; Astronomy; Telescope; Stars; Galactic plane; Pulsar; Galaxy","score_opus":0.013104449311677748,"score_gpt":0.2299798644580082,"score_spread":0.21687541514633044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153535686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979748,0.00007324297,0.00014480246,0.000021288206,0.0000014447938,0.000006395299,0.00097178743,0.000010294058,0.00079585507],"genre_scores_gemma":[0.9975534,0.00005203392,0.00035671785,0.00001969102,0.000005736259,0.000008472016,0.0017491715,0.0000044271787,0.00025036663],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998393,0.000020105568,0.0000095915775,0.000038449423,0.000045041616,0.000047471138],"domain_scores_gemma":[0.9995627,0.000047528618,0.00011729682,0.000039635404,0.00005312749,0.00017974597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025068986,0.00014981025,0.00026355474,0.0012298591,0.00044642793,0.0005431196,0.00028244578,0.00014243118,0.00051712873],"category_scores_gemma":[0.0005002062,0.00019107242,0.00023712897,0.00072090677,0.00025829265,0.00017506754,0.0008221846,0.00024168426,0.00018289809],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010179315,0.00003559657,0.9782205,0.00001793315,0.00004723341,0.00012213746,0.00020672439,0.0005906353,0.016069924,0.00023135636,0.00042752546,0.003928586],"study_design_scores_gemma":[0.0000068503855,0.000009603274,0.9986136,0.0000035427863,0.0000041101944,0.000044900244,0.000057737685,0.0004143118,0.0004003889,0.000020514959,0.000422641,0.0000018768499],"about_ca_topic_score_codex":0.01592569,"about_ca_topic_score_gemma":0.025670558,"teacher_disagreement_score":0.01592569,"about_ca_system_score_codex":0.000479152,"about_ca_system_score_gemma":0.0003495299,"threshold_uncertainty_score":0.03166604},"labels":[],"label_agreement":null},{"id":"W2153585063","doi":"10.1088/0004-637x/710/1/540","title":"SEARCHES FOR HIGH-FREQUENCY VARIATIONS IN THE<sup>8</sup>B SOLAR NEUTRINO FLUX AT THE SUDBURY NEUTRINO OBSERVATORY","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Sudbury; University of British Columbia; University of Guelph; Laurentian University; University of Alberta; Queen's University; TRIUMF; Carleton University","funders":"Science and Technology Facilities Council","keywords":"Physics; Observatory; Solar neutrino; Neutrino; Amplitude; Flux (metallurgy); Solar neutrino problem; Astrophysics; Satellite; Solar observatory; Neutrino oscillation; Astronomy; Particle physics; Optics","score_opus":0.029716937098959475,"score_gpt":0.2851357007138826,"score_spread":0.25541876361492316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153585063","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950564,0.0003902375,0.00063733564,0.00020683801,0.000011705394,0.000015559019,0.0005840383,0.00003231257,0.0030655048],"genre_scores_gemma":[0.9952891,0.00016762417,0.0028456172,0.00011715319,0.000025443394,0.0000096495,0.0008200374,0.000013497019,0.00071200775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993319,0.00013438324,0.000033126627,0.00015692363,0.00018888789,0.00015470468],"domain_scores_gemma":[0.99807835,0.00066307676,0.00050996075,0.000143985,0.00028694322,0.00031770414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012724439,0.00032329623,0.0004212975,0.0019713081,0.0013783808,0.0011912709,0.00068363524,0.0005527739,0.002136589],"category_scores_gemma":[0.0014469395,0.00037311492,0.00038450444,0.0013812911,0.00050067506,0.0004929956,0.00085690717,0.0004917076,0.0003192742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014005661,0.00016864568,0.74006766,0.00013917868,0.00053190405,0.0016618127,0.000648417,0.0013666954,0.21552554,0.001718743,0.0020990085,0.03467177],"study_design_scores_gemma":[0.00017608752,0.00045451935,0.9171092,0.000046250174,0.00025512133,0.0013520009,0.0005591332,0.0031792708,0.06629479,0.0009584224,0.009514029,0.00010114325],"about_ca_topic_score_codex":0.016227145,"about_ca_topic_score_gemma":0.04247829,"teacher_disagreement_score":0.016227145,"about_ca_system_score_codex":0.0006898991,"about_ca_system_score_gemma":0.00074660295,"threshold_uncertainty_score":0.032265425},"labels":[],"label_agreement":null},{"id":"W2153615851","doi":"10.1088/0004-637x/787/1/51","title":"REALISTIC MODELING OF THE PULSE PROFILE OF PSR J0737-3039A","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Neutron star; Magnetosphere; Millisecond pulsar; Pulse (music); Dipole; X-ray pulsar; Binary pulsar; Magnetic dipole","score_opus":0.014594696282305886,"score_gpt":0.30148275226935295,"score_spread":0.2868880559870471,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153615851","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96608925,0.00013389022,0.024101753,0.00023328743,0.000033897588,0.000045420802,0.0017979969,0.00031665905,0.007247877],"genre_scores_gemma":[0.9938222,0.00006647492,0.0046197497,0.00003133176,0.0000068864433,0.000034101828,0.0007159228,0.00004621966,0.000657088],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994314,0.000011931914,0.0000035386065,0.000018758616,0.000010744608,0.000011919199],"domain_scores_gemma":[0.9998652,0.000045889752,0.000027541952,0.000017129081,0.000022382246,0.000021830385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012195844,0.0002492337,0.00019015677,0.00023354118,0.00024570027,0.0004516532,0.00048528024,0.0005551621,0.0011332332],"category_scores_gemma":[0.000454578,0.00021419286,0.00029643322,0.00037771443,0.00020142451,0.00029563,0.00022202289,0.00035608388,0.00023852008],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015144938,0.00009087063,0.015596533,0.00005877532,0.000050709023,0.00027316975,0.00016448835,0.9518023,0.019896943,0.0051327148,0.0010265561,0.0057553975],"study_design_scores_gemma":[0.000038275666,0.0000418932,0.011048974,0.000005500173,0.000017077013,0.0001012556,0.000040851075,0.98441213,0.0021160534,0.0009172469,0.001236807,0.000023961851],"about_ca_topic_score_codex":0.010049736,"about_ca_topic_score_gemma":0.007115864,"teacher_disagreement_score":0.010049736,"about_ca_system_score_codex":0.00059048977,"about_ca_system_score_gemma":0.00046431614,"threshold_uncertainty_score":0.019982457},"labels":[],"label_agreement":null},{"id":"W2153887579","doi":"10.1086/512477","title":"The Environment of Local Ultraluminous Infrared Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"QSOS; Physics; Astrophysics; Luminous infrared galaxy; Galaxy; Field galaxy; Astronomy; Redshift; Luminosity; Population; Redshift survey","score_opus":0.005225411576720628,"score_gpt":0.19404482486641145,"score_spread":0.18881941328969082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153887579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99946886,0.00003109235,0.00006528355,0.0000031773861,1.85396e-7,0.0000012386124,0.00015193364,0.000005565818,0.00027261497],"genre_scores_gemma":[0.9993326,0.000025536776,0.00007675707,0.0000014875914,9.4718075e-7,0.0000014891073,0.000485834,0.000001685498,0.00007360461],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997844,0.000026764275,0.000009990822,0.00007133411,0.000038783757,0.000068757356],"domain_scores_gemma":[0.99904245,0.00015438741,0.0004200068,0.00012711535,0.000091910915,0.00016398038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002587087,0.00015407075,0.00028724296,0.0016400153,0.00029185743,0.0005840662,0.0002824086,0.00014562743,0.0008844336],"category_scores_gemma":[0.0009141693,0.000108385764,0.00021680933,0.0015350102,0.0003891484,0.00028374078,0.0006593038,0.00015227967,0.0001884949],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008374551,0.000021608015,0.98778874,0.000013265649,0.000060922484,0.00009162511,0.0001661173,0.002176053,0.0038023582,0.00033589598,0.00013675832,0.005323031],"study_design_scores_gemma":[0.0000016490366,0.000012959698,0.99837613,0.0000011621869,0.000009274306,0.00006151837,0.000060904604,0.0009842371,0.00030622876,0.000055424982,0.00012771529,0.0000027550718],"about_ca_topic_score_codex":0.0098075615,"about_ca_topic_score_gemma":0.009528559,"teacher_disagreement_score":0.0098075615,"about_ca_system_score_codex":0.00060569745,"about_ca_system_score_gemma":0.00019977617,"threshold_uncertainty_score":0.01950097},"labels":[],"label_agreement":null},{"id":"W2153931839","doi":"10.1086/590482","title":"AGN Dusty Tori. I. Handling of Clumpy Media","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":608,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Seneca Polytechnic","funders":"","keywords":"Physics; Torus; Astrophysics; Radiative transfer; Active galactic nucleus; Radiation; Formalism (music); Galaxy; Geometry; Optics","score_opus":0.011603372064466074,"score_gpt":0.20818136207984178,"score_spread":0.1965779900153757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153931839","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.11640563,0.002596337,0.86267877,0.0007475223,0.00032798437,0.00021020435,0.00053539785,0.00091163995,0.015586583],"genre_scores_gemma":[0.835323,0.0019564452,0.15296799,0.00021673008,0.00051406556,0.0002374603,0.00058239925,0.00015152048,0.0080505],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995104,0.0001093089,0.000042426105,0.000104872015,0.00014266034,0.000090384376],"domain_scores_gemma":[0.99891484,0.0002845643,0.00030010752,0.00031386223,0.00011103832,0.00007565716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006372505,0.0008174898,0.0008506212,0.00077419635,0.0011458566,0.0023508416,0.0017489977,0.0010047609,0.0016278373],"category_scores_gemma":[0.0029935818,0.00041985637,0.0011541437,0.00062787224,0.0014411947,0.002292593,0.0024917298,0.0011897582,0.00046329774],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027513845,0.000083488594,0.0176039,0.0006828224,0.0001432398,0.008080333,0.001296242,0.15894994,0.034560844,0.6937031,0.005827774,0.07879314],"study_design_scores_gemma":[0.000076267526,0.00011948335,0.0056623598,0.00010906612,0.00010780174,0.0056742923,0.001005896,0.62048966,0.0142358765,0.31189185,0.04051983,0.000107631306],"about_ca_topic_score_codex":0.0021969175,"about_ca_topic_score_gemma":0.0016790552,"teacher_disagreement_score":0.0023508416,"about_ca_system_score_codex":0.00079357746,"about_ca_system_score_gemma":0.00048808972,"threshold_uncertainty_score":0.0057578087},"labels":[],"label_agreement":null},{"id":"W2153956945","doi":"10.1086/529402","title":"Mass and Redshift Dependence of Star Formation in Relaxed Galaxy Clusters","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Astrophysics; Physics; Velocity dispersion; Redshift; Galaxy cluster; Star formation; Cluster (spacecraft); Galaxy; Stellar mass; Astronomy; Luminosity; Star cluster","score_opus":0.009182365954375991,"score_gpt":0.20465221292729,"score_spread":0.195469846972914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2153956945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962556,0.000042371954,0.00005212779,0.0000044512544,2.4071701e-7,0.0000010658191,0.0001346989,0.000006197094,0.00013328051],"genre_scores_gemma":[0.9994362,0.000017489392,0.00005275676,0.0000017256455,9.419818e-7,9.680429e-7,0.00041236804,0.0000021986302,0.000075275304],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983525,0.000023582215,0.000012169604,0.000053149986,0.000032875578,0.000042904387],"domain_scores_gemma":[0.99720865,0.00062093086,0.0013002137,0.0002617815,0.00029949896,0.0003089056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033404474,0.00015150452,0.00021033263,0.0013072914,0.0002125993,0.00040486862,0.00024483222,0.0001780564,0.00087746367],"category_scores_gemma":[0.0025676554,0.00013639222,0.00023415592,0.0008347108,0.00027757778,0.00028691755,0.0003904635,0.00016024178,0.00018204971],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016397412,0.000009791188,0.991385,0.000010203055,0.00005852725,0.000045031473,0.00016770551,0.0014977817,0.004418172,0.000121895086,0.000059805003,0.0020622015],"study_design_scores_gemma":[0.0000019610063,0.00001544992,0.9989467,9.922488e-7,0.000004909326,0.000034647674,0.00002313083,0.00070110644,0.00018525793,0.000026936686,0.000056669596,0.0000022514846],"about_ca_topic_score_codex":0.007144839,"about_ca_topic_score_gemma":0.008070767,"teacher_disagreement_score":0.007144839,"about_ca_system_score_codex":0.00034672927,"about_ca_system_score_gemma":0.00009112873,"threshold_uncertainty_score":0.014206529},"labels":[],"label_agreement":null},{"id":"W2154051073","doi":"10.1086/382703","title":"The Evolution of the Accretion Disk around 4U 1820-30 during a Superburst","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Neutron star; Physics; Astrophysics; Accretion (finance); RADIUS; Intermediate polar; Accretion disc; Ionization; Astronomy; Thick disk; Stars; White dwarf; Galaxy; Ion","score_opus":0.007253153233560928,"score_gpt":0.21028836321755034,"score_spread":0.2030352099839894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154051073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99876106,0.0001419822,0.0001011419,0.000025696574,0.000005953687,0.000004531867,0.000076213946,0.000014599456,0.0008688336],"genre_scores_gemma":[0.9988281,0.00007530264,0.0003561677,0.000022516266,0.000006525834,0.0000053140698,0.00027407362,0.0000111474865,0.00042076918],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999553,0.000004670309,0.0000023169546,0.000015568574,0.000010471531,0.000011666263],"domain_scores_gemma":[0.99982625,0.000021343181,0.000051290826,0.000014334492,0.00002410969,0.00006277174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013698082,0.00025249156,0.00038121975,0.00048297585,0.00051619654,0.00049813755,0.0003247066,0.0004107524,0.0005663653],"category_scores_gemma":[0.00032002782,0.00026373926,0.0001984527,0.0003537892,0.0003542274,0.00026610846,0.0005282794,0.00041328953,0.00029265461],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00173584,0.00028172776,0.359424,0.00018848815,0.00017957798,0.0074240207,0.0017601287,0.0061490764,0.6030066,0.0008294404,0.0010518893,0.017969156],"study_design_scores_gemma":[0.000034770153,0.00018010389,0.9854914,0.000015108027,0.00002645204,0.0005846088,0.00030364413,0.004157397,0.007686752,0.00016441238,0.0013369904,0.000018240919],"about_ca_topic_score_codex":0.005432459,"about_ca_topic_score_gemma":0.0065066977,"teacher_disagreement_score":0.005432459,"about_ca_system_score_codex":0.0007191861,"about_ca_system_score_gemma":0.00018662715,"threshold_uncertainty_score":0.010801673},"labels":[],"label_agreement":null},{"id":"W2154075011","doi":"10.1086/589152","title":"New Results on the Submillimeter Polarization Spectrum of the Orion Molecular Cloud","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Polarimeter; Polarization (electrochemistry); Molecular cloud; Wavelength; Astrophysics; Astronomy; Orion Nebula; Polarimetry; Infrared; Optics; Stars; Chemistry","score_opus":0.010715862073546793,"score_gpt":0.21102316684572914,"score_spread":0.20030730477218234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154075011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96856135,0.0014650215,0.008169469,0.00029592414,0.00008796405,0.000022557024,0.0041628606,0.0003320248,0.016902909],"genre_scores_gemma":[0.9817523,0.00065076485,0.011497147,0.00013242138,0.00013395971,0.000021057469,0.0039062705,0.00006883,0.001837148],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979633,0.000016670867,0.0000056186555,0.00006425362,0.00006937403,0.000047742637],"domain_scores_gemma":[0.9996013,0.00007873167,0.00007192911,0.00008933174,0.00010511536,0.000053576277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039120065,0.0002330854,0.00014114125,0.0009495012,0.00030656674,0.0007475633,0.00027701334,0.00018974148,0.0028629575],"category_scores_gemma":[0.00053929485,0.00017871024,0.00020547639,0.0010306181,0.0001934126,0.0005464577,0.0003913991,0.0003664987,0.0004886136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006137685,0.00022312066,0.4254834,0.00018405163,0.00011837152,0.00084433827,0.0010339675,0.003156588,0.40938333,0.0045445026,0.0047632046,0.14965132],"study_design_scores_gemma":[0.000023923525,0.00006802957,0.9270774,0.00004194723,0.0000657684,0.0005710422,0.00015780028,0.0038769662,0.045172486,0.0018631067,0.021046331,0.000035172383],"about_ca_topic_score_codex":0.0027496351,"about_ca_topic_score_gemma":0.00520506,"teacher_disagreement_score":0.0028629575,"about_ca_system_score_codex":0.0002736734,"about_ca_system_score_gemma":0.00010668208,"threshold_uncertainty_score":0.009577572},"labels":[],"label_agreement":null},{"id":"W2154208465","doi":"10.1088/0004-637x/760/2/116","title":"MICROLENSING BINARIES WITH CANDIDATE BROWN DWARF COMPANIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Marsden Fund; Japan Society for the Promotion of Science; National Research Foundation of Korea; Fonds National de la Recherche Luxembourg; Qatar National Research Fund; Qatar Foundation; Korea Research Council of Fundamental Science and Technology; Fonds pour la Formation à la Recherche dans l’Industrie et dans l’Agriculture; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; California Institute of Technology; European Commission; Fédération Wallonie-Bruxelles; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Gravitational microlensing; Brown dwarf; Astrophysics; Astronomy; Binary star; Circumbinary planet; Stars","score_opus":0.010874048605068147,"score_gpt":0.21859073907485496,"score_spread":0.2077166904697868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154208465","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983772,0.00031316868,0.0002973239,0.000015638869,0.0000057046095,0.000006329397,0.00010963782,0.000028621882,0.00084645225],"genre_scores_gemma":[0.99909997,0.000045246474,0.00025585905,0.000014676427,0.000008681425,0.00000228522,0.00027520128,0.0000030005524,0.00029502605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977106,0.000013400969,0.000015834341,0.00006905854,0.000056378984,0.0000742424],"domain_scores_gemma":[0.9993051,0.00008331243,0.00035794504,0.00004494617,0.00004482554,0.00016382216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022633378,0.00026325564,0.00029464543,0.0015561478,0.0006506807,0.00086693745,0.00028563038,0.0002753295,0.0020326502],"category_scores_gemma":[0.000566252,0.00015003412,0.00020686166,0.0011609714,0.00023720427,0.0003600751,0.00077438785,0.00017459627,0.0004560146],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016444159,0.00003840834,0.979071,0.000022214885,0.00003983846,0.00089435745,0.00015862407,0.0001047178,0.009672603,0.00020246656,0.00022436668,0.0094070975],"study_design_scores_gemma":[0.00000783329,0.00004321346,0.9925206,0.000008220741,0.00003301324,0.0016394097,0.00031752716,0.0008802498,0.0028574788,0.00020969957,0.001476918,0.0000057725733],"about_ca_topic_score_codex":0.0027214668,"about_ca_topic_score_gemma":0.005623926,"teacher_disagreement_score":0.0027214668,"about_ca_system_score_codex":0.00040547867,"about_ca_system_score_gemma":0.00017955349,"threshold_uncertainty_score":0.0067998767},"labels":[],"label_agreement":null},{"id":"W2154229202","doi":"10.1088/0004-637x/730/2/112","title":"THE M33 GLOBULAR CLUSTER SYSTEM WITH PAndAS DATA: THE LAST OUTER HALO CLUSTER?","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics; McMaster University","funders":"Science and Technology Facilities Council","keywords":"Halo; Globular cluster; RADIUS; Cluster (spacecraft); Galactic halo; Star cluster; Galaxy","score_opus":0.014197370216877411,"score_gpt":0.20714930221884195,"score_spread":0.19295193200196453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154229202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99359375,0.00007269646,0.00026601763,0.00005914911,0.0000036843214,0.000015084972,0.004206464,0.000110816734,0.0016723328],"genre_scores_gemma":[0.98728186,0.000040007162,0.0024523993,0.00002022374,0.0000068351824,0.000011541143,0.009861882,0.000035493464,0.00028990966],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999793,0.000021589563,0.0000080187,0.00006362868,0.00004719175,0.00006665488],"domain_scores_gemma":[0.99959546,0.000017943988,0.00009819474,0.0001132261,0.000051560462,0.00012358336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028574342,0.00023178165,0.00018803823,0.0010061307,0.00042956538,0.0005508806,0.0003155169,0.00022875583,0.0015816295],"category_scores_gemma":[0.00059437996,0.00015416922,0.0002290328,0.0017673882,0.0001759659,0.00027178897,0.00084509683,0.00021355743,0.00071659015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036809625,0.00006587315,0.95563596,0.00005975461,0.00011119716,0.00029555822,0.000490478,0.002000882,0.0086643975,0.0008326464,0.006766515,0.024708621],"study_design_scores_gemma":[0.000019811507,0.00003565898,0.9864239,0.000010222861,0.000030420331,0.00015918014,0.00022755947,0.0035408027,0.0011374112,0.00015571533,0.008245031,0.000014272987],"about_ca_topic_score_codex":0.063107304,"about_ca_topic_score_gemma":0.09092649,"teacher_disagreement_score":0.063107304,"about_ca_system_score_codex":0.000529118,"about_ca_system_score_gemma":0.0005654212,"threshold_uncertainty_score":0.12548},"labels":[],"label_agreement":null},{"id":"W2154346895","doi":"10.1086/500577","title":"Two Populations of Young Massive Star Clusters in Arp 220","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Star cluster; Physics; Astrophysics; Globular cluster; Star formation; Luminosity; Galaxy; Cluster (spacecraft); Astronomy; Population; Demography","score_opus":0.008482875990791304,"score_gpt":0.22565650397974374,"score_spread":0.21717362798895243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154346895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994054,0.00006015444,0.00013857805,0.0000069870034,0.0000013483833,0.0000033067213,0.000050940696,0.000006804126,0.00032654864],"genre_scores_gemma":[0.99904746,0.000049072954,0.00033062816,0.000010543607,0.0000059449926,0.000004548509,0.00036944574,0.000003727999,0.00017863288],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973613,0.00003058995,0.000020082281,0.000087452274,0.000067046036,0.000058571408],"domain_scores_gemma":[0.99924636,0.00009727124,0.00028421334,0.000060814735,0.00007477023,0.00023658799],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034182175,0.00024831935,0.00033384768,0.0012924758,0.0008488945,0.001311779,0.0004410027,0.00031749243,0.00045012205],"category_scores_gemma":[0.0011910156,0.0003077677,0.00018779493,0.0005201036,0.00041750894,0.0004157323,0.0007800544,0.0002312016,0.00017052983],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003600292,0.00008369093,0.98155105,0.000021376498,0.000042856987,0.00028589217,0.0010456385,0.0008233785,0.007961797,0.0006292841,0.00018972323,0.007005378],"study_design_scores_gemma":[0.000015455991,0.00010861833,0.9948207,0.000006659659,0.000032100077,0.0008853815,0.00036900694,0.0013570379,0.0011582702,0.00035973755,0.00086269237,0.000024256326],"about_ca_topic_score_codex":0.0034299786,"about_ca_topic_score_gemma":0.004742228,"teacher_disagreement_score":0.0034299786,"about_ca_system_score_codex":0.0005013967,"about_ca_system_score_gemma":0.00017777836,"threshold_uncertainty_score":0.006820023},"labels":[],"label_agreement":null},{"id":"W2154415107","doi":"10.1088/0004-637x/691/2/1109","title":"ON THE DYNAMICAL EVOLUTION OF H II REGIONS: AN INVESTIGATION OF THE IONIZED COMPONENT OF W4, A GALACTIC CHIMNEY CANDIDATE. I. KINEMATICS AND DYNAMICS IN THE LATITUDE RANGE 0° ⩽<i>b</i>⩽ 3°","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Astronomy; Nebula; Superbubble; Galaxy; Molecular cloud; Galactic Center; Redshift; Milky Way; H II region; Interstellar medium; Star formation; Stars","score_opus":0.009403281121240612,"score_gpt":0.22733176274536993,"score_spread":0.2179284816241293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154415107","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997662,0.000020050216,0.000025835894,0.0000051173834,1.9494088e-7,0.0000012559059,0.000020242094,0.0000013920993,0.00015966558],"genre_scores_gemma":[0.99944395,0.000035088695,0.00014396547,0.0000083448485,0.0000017753845,0.00000199609,0.00014999736,0.000001585562,0.00021329866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996483,0.000004018087,0.0000014859695,0.000008987665,0.000008052305,0.000012631212],"domain_scores_gemma":[0.9998846,0.000012427734,0.000042629563,0.0000053349618,0.000017242306,0.000037623897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000100200064,0.00016225639,0.00008342401,0.0006138143,0.00035944523,0.00028914431,0.0002753623,0.00018000792,0.0005696176],"category_scores_gemma":[0.00017050318,0.00008569326,0.00009482388,0.0002873216,0.00023776354,0.00021686968,0.00032968752,0.00013670615,0.000180667],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012046946,0.000034886878,0.9615213,0.000009637211,0.000021172416,0.00046964933,0.000424398,0.00012419878,0.033093713,0.0000718316,0.00007473495,0.004034017],"study_design_scores_gemma":[0.0000021233143,0.0000754284,0.99693215,0.0000014870627,0.00000822971,0.0002678996,0.0003722849,0.00025791285,0.0016220058,0.00002561107,0.00043286415,0.0000019629658],"about_ca_topic_score_codex":0.007799934,"about_ca_topic_score_gemma":0.013584763,"teacher_disagreement_score":0.007799934,"about_ca_system_score_codex":0.0002826947,"about_ca_system_score_gemma":0.000116526666,"threshold_uncertainty_score":0.015509069},"labels":[],"label_agreement":null},{"id":"W2154564705","doi":"10.1088/0004-637x/697/2/1827","title":"STABILITY OF A SPHERICAL ACCRETION SHOCK WITH NUCLEAR DISSOCIATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Shock wave; Instability; Accretion (finance); Shock (circulatory); Adiabatic process; Amplitude; Neutrino; Equation of state","score_opus":0.006473019149213956,"score_gpt":0.20807901189328967,"score_spread":0.20160599274407573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154564705","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933068,0.000047510974,0.0039458913,0.00011169601,0.000011143889,0.00001320411,0.00003319772,0.00004815513,0.002482387],"genre_scores_gemma":[0.99848324,0.00003882367,0.0007062363,0.000029172741,0.000008423893,0.000007754299,0.00005216121,0.00001264622,0.00066138315],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988663,0.000019187164,0.0000063603543,0.0000145595795,0.000028234092,0.000045041685],"domain_scores_gemma":[0.9995881,0.0001012245,0.00011160496,0.000022090271,0.00005767532,0.000119300494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028868267,0.0004383702,0.0003577302,0.0005250686,0.0005501696,0.0010400271,0.000586262,0.00068555307,0.0009770497],"category_scores_gemma":[0.0013805703,0.00022153274,0.0005807885,0.00029146508,0.0012359592,0.00050437753,0.001292117,0.00053617137,0.0001368281],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006076963,0.00017544434,0.018028125,0.0000931252,0.00013263215,0.0014152451,0.00053901586,0.8900675,0.060050707,0.02318571,0.00053325004,0.0051714275],"study_design_scores_gemma":[0.00003199542,0.00007525685,0.0026385516,0.000003628086,0.00000968012,0.00005850639,0.00006829903,0.99283385,0.0029181603,0.0012460295,0.00010188809,0.000014182291],"about_ca_topic_score_codex":0.008190001,"about_ca_topic_score_gemma":0.0017509068,"teacher_disagreement_score":0.008190001,"about_ca_system_score_codex":0.0007372487,"about_ca_system_score_gemma":0.0007352774,"threshold_uncertainty_score":0.016284645},"labels":[],"label_agreement":null},{"id":"W2154577062","doi":"10.1086/431294","title":"Observations of the BL Lacertae Object 3C 66A with STACEE","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; TRIUMF; McGill University","funders":"","keywords":"Physics; BL Lac object; Astrophysics; Tower; Flux (metallurgy); Gamma ray; Geography","score_opus":0.011448070992169926,"score_gpt":0.2118948525857773,"score_spread":0.20044678159360738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154577062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965712,0.00033928922,0.0003898092,0.00004452739,0.000007175769,0.000013761817,0.0010224812,0.00006516055,0.0015466188],"genre_scores_gemma":[0.99288577,0.00033327495,0.0022124366,0.000051553965,0.000029714756,0.000010722643,0.0036921958,0.000027410331,0.0007569639],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996556,0.000024221763,0.000013092233,0.000070767164,0.00014909032,0.0000872597],"domain_scores_gemma":[0.99898154,0.00009279855,0.00030389454,0.00022657108,0.00018697491,0.00020818494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005638234,0.000345348,0.0003654212,0.0024350584,0.0007218534,0.0007083717,0.00034318972,0.0005049266,0.00081160414],"category_scores_gemma":[0.00079820986,0.00028845322,0.0003849095,0.0027497332,0.00037731283,0.00044654877,0.00091708405,0.00049080286,0.0004275805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016679582,0.0003946747,0.8390755,0.0002318001,0.00035117075,0.002541849,0.0012816543,0.0027432744,0.09392011,0.0007876259,0.0030838551,0.053920515],"study_design_scores_gemma":[0.00004144449,0.00013470033,0.98548514,0.000012309102,0.000042026466,0.00088422035,0.000090075024,0.0011833214,0.0052555115,0.000105917235,0.0067376574,0.000027716089],"about_ca_topic_score_codex":0.0077938326,"about_ca_topic_score_gemma":0.029111795,"teacher_disagreement_score":0.0077938326,"about_ca_system_score_codex":0.00054281036,"about_ca_system_score_gemma":0.00024938988,"threshold_uncertainty_score":0.015496969},"labels":[],"label_agreement":null},{"id":"W2154655514","doi":"10.1088/0004-637x/742/2/85","title":"THE EXTREME SPIN OF THE BLACK HOLE IN CYGNUS X-1","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":266,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Black hole (networking); Spin-flip; Rotating black hole; Binary black hole; Angular momentum; Stellar black hole; Intermediate-mass black hole; X-ray binary","score_opus":0.033007662761855204,"score_gpt":0.2299809013550625,"score_spread":0.19697323859320728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154655514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99945813,0.000047288104,0.00013713849,0.00001303885,0.0000018444182,7.871416e-7,0.000010131133,0.0000041539643,0.00032757182],"genre_scores_gemma":[0.99981016,0.000015742493,0.000102912425,0.0000058934047,0.0000021593032,7.28934e-7,0.000019166622,0.0000015179111,0.00004182461],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991405,0.000015295587,0.0000033113874,0.000033910674,0.00001653784,0.000016790396],"domain_scores_gemma":[0.99968624,0.000057088953,0.00016685468,0.000023611532,0.000021842616,0.00004448866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029773923,0.00017962763,0.00019579992,0.0004893666,0.00047579056,0.00069111853,0.00019543231,0.00026003987,0.00027798722],"category_scores_gemma":[0.0011430265,0.00013084938,0.000071263086,0.00020000011,0.0007323341,0.00029513575,0.0006510523,0.000230036,0.000073206866],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009736275,0.000051324863,0.821005,0.00006645377,0.00007622554,0.0023729831,0.0010651051,0.009239344,0.14308126,0.007932392,0.00035626415,0.013780007],"study_design_scores_gemma":[0.000037210713,0.00017407848,0.96882635,0.000027287568,0.00003150142,0.00092740223,0.00029232254,0.013015099,0.012744561,0.0031170666,0.0007742184,0.00003290793],"about_ca_topic_score_codex":0.0019147497,"about_ca_topic_score_gemma":0.0023849302,"teacher_disagreement_score":0.0019147497,"about_ca_system_score_codex":0.00043574,"about_ca_system_score_gemma":0.00013952827,"threshold_uncertainty_score":0.003807187},"labels":[],"label_agreement":null},{"id":"W2154768789","doi":"10.1088/0004-637x/793/1/40","title":"HIghMass-HIGH H I MASS, H I-RICH GALAXIES AT<i>z</i>∼ 0 SAMPLE DEFINITION, OPTICAL AND Hα IMAGING, AND STAR FORMATION PROPERTIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Galaxy; Star formation; Luminosity; Surface brightness; Halo; Dark matter; Brightness; Galaxy formation and evolution","score_opus":0.008804000171222954,"score_gpt":0.18410769893270834,"score_spread":0.17530369876148538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154768789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972097,0.000048485577,0.00015729296,0.000013229558,0.0000011665834,0.000009953296,0.0014601136,0.000012684409,0.0010872344],"genre_scores_gemma":[0.9959079,0.000029357447,0.00022573379,0.000022483648,0.000007477832,0.000014447643,0.003242263,0.00000527538,0.0005450113],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970347,0.000027907867,0.000028911196,0.00007624565,0.000061358536,0.000102071346],"domain_scores_gemma":[0.9991047,0.00011718796,0.00029255153,0.00012738322,0.00009598567,0.00026217924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038293828,0.0002064459,0.00018921483,0.0014717921,0.00033479018,0.0006332763,0.00020719465,0.00015761591,0.0028459353],"category_scores_gemma":[0.0009197465,0.000083253944,0.00017572983,0.00087341934,0.00022972147,0.00027344283,0.0007078774,0.00012272665,0.00076027313],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005615982,0.000023787414,0.9943235,0.000006822049,0.000013087476,0.000064366184,0.000117652795,0.000031675332,0.0021382596,0.000084527994,0.00020232244,0.0029377094],"study_design_scores_gemma":[0.0000015193092,0.000018443481,0.9990928,0.000001150994,0.000005155014,0.00015166847,0.00009641389,0.00003680497,0.00025493387,0.00002148443,0.0003186552,7.4348145e-7],"about_ca_topic_score_codex":0.0024457634,"about_ca_topic_score_gemma":0.0042446353,"teacher_disagreement_score":0.0028459353,"about_ca_system_score_codex":0.00017687444,"about_ca_system_score_gemma":0.00014715381,"threshold_uncertainty_score":0.00952065},"labels":[],"label_agreement":null},{"id":"W2154811628","doi":"10.1088/0004-637x/710/1/634","title":"MAGIC GAMMA-RAY TELESCOPE OBSERVATION OF THE PERSEUS CLUSTER OF GALAXIES: IMPLICATIONS FOR COSMIC RAYS, DARK MATTER, AND NGC 1275","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":152,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Dark matter; Galaxy cluster; Cosmic ray; Fermi Gamma-ray Space Telescope; Astronomy; Galaxy; Spectral index; Spectral line","score_opus":0.010477887463268547,"score_gpt":0.22988606814184578,"score_spread":0.21940818067857723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154811628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980331,0.000060899474,0.00009201748,0.000048919355,0.0000030435947,0.0000038121166,0.00051884307,0.00002325566,0.0012160813],"genre_scores_gemma":[0.99901533,0.000029525732,0.00021560685,0.000013862247,0.000006440583,0.0000028542706,0.00054675224,0.0000033742622,0.00016619673],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999881,0.000017819457,0.0000044648596,0.00004220708,0.000028424456,0.00002614636],"domain_scores_gemma":[0.9996568,0.000036416775,0.00010711441,0.00003564171,0.00003761074,0.00012637409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002740823,0.00032469796,0.00020311843,0.0012365244,0.00033417888,0.0004102229,0.0003131375,0.00017097677,0.00076977874],"category_scores_gemma":[0.0004444369,0.00013727699,0.00016758738,0.0008772305,0.00033967366,0.00018197492,0.00066736504,0.00020624128,0.00017145657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014576362,0.000028359374,0.9854176,0.000012324831,0.000046542853,0.00038526198,0.00028917185,0.00039982318,0.0067198384,0.0003347575,0.0008055558,0.005415061],"study_design_scores_gemma":[0.0000052422606,0.000015275422,0.99874437,0.0000028182574,0.0000064387013,0.0000920038,0.00008231287,0.00031302104,0.00025349943,0.000041013285,0.0004409743,0.0000030380297],"about_ca_topic_score_codex":0.025492882,"about_ca_topic_score_gemma":0.031608723,"teacher_disagreement_score":0.025492882,"about_ca_system_score_codex":0.0007057203,"about_ca_system_score_gemma":0.00028924167,"threshold_uncertainty_score":0.050688982},"labels":[],"label_agreement":null},{"id":"W2154817990","doi":"10.1088/0004-637x/779/2/94","title":"GLOBULAR CLUSTER SCALE SIZES IN GIANT GALAXIES: THE CASE OF M87 AND THE ROLE OF ORBITAL ANISOTROPY AND TIDAL FILLING","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Anisotropy; Cluster (spacecraft); Galaxy; Isotropy; Population; Quantum mechanics","score_opus":0.0031886842544800497,"score_gpt":0.18661415525309658,"score_spread":0.18342547099861653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154817990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99755836,0.000228941,0.00032517145,0.00014762058,0.0000022595375,0.0000030216695,0.000043950382,0.000012966668,0.0016777412],"genre_scores_gemma":[0.99957985,0.000087538305,0.00017097002,0.000008380855,0.000004330104,0.0000017412839,0.000023322551,0.0000066169982,0.00011720569],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998598,0.000047370177,0.0000055507426,0.00002223783,0.000018975095,0.000046058918],"domain_scores_gemma":[0.9978023,0.0011938945,0.0004563662,0.00018671644,0.000098771154,0.00026192737],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061892543,0.00021057425,0.0002523943,0.0009439178,0.00056311605,0.0010474514,0.00090207567,0.0005602014,0.00067433866],"category_scores_gemma":[0.004774869,0.00017930745,0.00034677886,0.00068553805,0.0016107421,0.0006362755,0.0007555013,0.00034768952,0.00008743877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035284326,0.00012433955,0.5938229,0.00010399922,0.00016213054,0.0020135327,0.001793736,0.3280328,0.0050658933,0.052280337,0.0026472714,0.013600205],"study_design_scores_gemma":[0.00008642412,0.00012157851,0.46924257,0.00005435269,0.00015835262,0.0004960864,0.0012890076,0.5046405,0.0016186107,0.02033789,0.0018888984,0.00006564394],"about_ca_topic_score_codex":0.0526612,"about_ca_topic_score_gemma":0.062142506,"teacher_disagreement_score":0.0526612,"about_ca_system_score_codex":0.0015108464,"about_ca_system_score_gemma":0.00042851697,"threshold_uncertainty_score":0.10470939},"labels":[],"label_agreement":null},{"id":"W2154944160","doi":"10.1088/0004-637x/772/1/37","title":"THE C-FLAME QUENCHING BY CONVECTIVE BOUNDARY MIXING IN SUPER-AGB STARS AND THE FORMATION OF HYBRID C/O/Ne WHITE DWARFS AND SN PROGENITORS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Convection; Stars; Supernova; Mixing (physics); White dwarf; Convective mixing; Stellar evolution; Thermonuclear fusion; Convection zone","score_opus":0.004126907920042793,"score_gpt":0.1966279228996289,"score_spread":0.1925010149795861,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2154944160","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99787474,0.00006760358,0.0007477517,0.000036906684,0.0000066135335,0.0000049380305,0.000034978217,0.000027222053,0.0011991699],"genre_scores_gemma":[0.9994312,0.000026424335,0.00023713056,0.000009281504,0.0000027866909,0.0000032244216,0.000036327572,0.000013182597,0.00024057373],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993587,0.000011064358,0.0000037974619,0.000012965594,0.000012489645,0.000023809449],"domain_scores_gemma":[0.9997539,0.000032423653,0.00007404986,0.000011890742,0.000021947186,0.00010581156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019300915,0.00048411268,0.00039326577,0.00031132618,0.0005106267,0.0008210412,0.0004803675,0.00048500602,0.0011034554],"category_scores_gemma":[0.0005254546,0.00035121554,0.0006075039,0.00018273127,0.0005780421,0.00036886946,0.0007247018,0.00036979845,0.00018196415],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00177642,0.0005350616,0.14026247,0.00018460029,0.00033578975,0.002558402,0.0006866783,0.56987363,0.25473827,0.0199524,0.0009529503,0.008143328],"study_design_scores_gemma":[0.00039450394,0.00034267595,0.09404555,0.00002102343,0.00008012235,0.00025008465,0.00023808939,0.8813629,0.016674642,0.0055894535,0.000938865,0.00006195965],"about_ca_topic_score_codex":0.009126953,"about_ca_topic_score_gemma":0.0035097501,"teacher_disagreement_score":0.009126953,"about_ca_system_score_codex":0.0009433667,"about_ca_system_score_gemma":0.00043824772,"threshold_uncertainty_score":0.018147647},"labels":[],"label_agreement":null},{"id":"W2155008346","doi":"10.1086/591271","title":"Connecting Substructure in Galaxy Cluster Cores at <i>z</i> = 0.2 with Cluster Assembly Histories","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Substructure; Astrophysics; Physics; Cluster (spacecraft); Galaxy cluster; Galaxy; Structure formation; Gravitational lens; Weak gravitational lensing; Brightest cluster galaxy; Redshift","score_opus":0.007378345449817077,"score_gpt":0.1968935122735685,"score_spread":0.1895151668237514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155008346","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980592,0.000042444615,0.00085550995,0.00003848697,0.0000014088074,0.0000051687125,0.00027329987,0.00005010388,0.00067430467],"genre_scores_gemma":[0.9992379,0.000016476835,0.00036448397,0.0000065123318,0.000002242811,0.0000025750494,0.00028327087,0.000007507058,0.00007897605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990976,0.000013447127,0.0000039018664,0.00003332232,0.000015052242,0.00002451431],"domain_scores_gemma":[0.99884254,0.000285236,0.0004842463,0.00011465596,0.00011956493,0.00015382982],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044939638,0.00036539594,0.0001311008,0.0009454213,0.00018842967,0.00080133113,0.00048361227,0.00035600172,0.0007232608],"category_scores_gemma":[0.002542465,0.00035037595,0.00041440796,0.00054155197,0.00038230064,0.00055482116,0.00062960916,0.000315885,0.00020330114],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020709303,0.000029567447,0.9433798,0.000024399647,0.0001009622,0.00013931932,0.00028645853,0.042570904,0.0073075388,0.0016414381,0.00030747583,0.0040050982],"study_design_scores_gemma":[0.000015512105,0.000041985502,0.8938588,0.000008761682,0.00004740452,0.000117541334,0.00014450567,0.10089058,0.0028206531,0.001616313,0.00041279645,0.000025262405],"about_ca_topic_score_codex":0.018522052,"about_ca_topic_score_gemma":0.012388351,"teacher_disagreement_score":0.018522052,"about_ca_system_score_codex":0.0011672032,"about_ca_system_score_gemma":0.00022481513,"threshold_uncertainty_score":0.03682846},"labels":[],"label_agreement":null},{"id":"W2155061646","doi":"10.1088/0004-637x/762/1/59","title":"HerMES: CANDIDATE GRAVITATIONALLY LENSED GALAXIES AND LENSING STATISTICS AT SUBMILLIMETER WAVELENGTHS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":183,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Redshift; Gravitational lens; Flux (metallurgy); Weak gravitational lensing; Dark matter; Strong gravitational lensing; Source counts","score_opus":0.008950710798667726,"score_gpt":0.21873543656479946,"score_spread":0.20978472576613175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155061646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9817671,0.00039689842,0.0007630722,0.000106316314,0.000005991319,0.000011790965,0.013854961,0.00016442472,0.002929549],"genre_scores_gemma":[0.98490345,0.00016913374,0.0006752246,0.000031893753,0.000030426496,0.000012516816,0.012631137,0.000024300283,0.0015218437],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997311,0.000038563943,0.00001986524,0.00007086362,0.00007359892,0.00006583218],"domain_scores_gemma":[0.9979551,0.0005349253,0.0008906991,0.0001727633,0.00012371328,0.00032278622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007316365,0.00029855646,0.00030754448,0.0024044502,0.0001951366,0.00058891013,0.0003679109,0.00019433783,0.0076213432],"category_scores_gemma":[0.0022146683,0.00012585297,0.00032415203,0.0011978472,0.000168382,0.00039016028,0.00042909864,0.00017710819,0.0013914813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000098159675,0.000016729951,0.98847616,0.000020603207,0.00006505027,0.00008302309,0.000038757036,0.00058352406,0.0012598117,0.00033670978,0.0024312276,0.0065903496],"study_design_scores_gemma":[0.0000071741983,0.000024908559,0.99592173,0.0000051275056,0.000020055288,0.00021966251,0.00004588495,0.0011875965,0.0004898308,0.000182762,0.0018884965,0.0000067499045],"about_ca_topic_score_codex":0.0029293797,"about_ca_topic_score_gemma":0.003930623,"teacher_disagreement_score":0.0076213432,"about_ca_system_score_codex":0.00019126784,"about_ca_system_score_gemma":0.00014836606,"threshold_uncertainty_score":0.025495946},"labels":[],"label_agreement":null},{"id":"W2155099801","doi":"10.1088/0004-637x/762/2/114","title":"ON THE UNUSUAL GAS COMPOSITION IN THE β PICTORIS DEBRIS DISK","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Outgassing; Debris; Gas composition; Debris disk; Oxygen; Abundance of the chemical elements; Abundance (ecology); Chemical composition; Carbon fibers","score_opus":0.012884331242291826,"score_gpt":0.2449445615320423,"score_spread":0.23206023028975048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155099801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99591917,0.00071682164,0.00032868318,0.00007643451,0.000010504129,0.0000037457517,0.00012740353,0.000032699907,0.0027845318],"genre_scores_gemma":[0.99924064,0.00023060128,0.00018557788,0.000018689778,0.00002195463,0.0000028866314,0.00007729489,0.000005029345,0.00021741509],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999646,0.0000049390937,0.0000017030939,0.000015280862,0.0000048284037,0.000008572637],"domain_scores_gemma":[0.9998945,0.00002925482,0.00003714192,0.000009237333,0.0000071635773,0.000022599064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000077825454,0.0002164747,0.00014672942,0.0007935578,0.00038650108,0.000602122,0.00024395657,0.00021220885,0.00093088043],"category_scores_gemma":[0.00027826565,0.0001354815,0.00009705735,0.00042411452,0.00048503422,0.00027434924,0.00031244033,0.00016484744,0.00023205871],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096205086,0.00010993093,0.7489729,0.00020999732,0.00012712031,0.013374873,0.0009766401,0.005838922,0.19796947,0.0046090623,0.0016222376,0.025226843],"study_design_scores_gemma":[0.000041332616,0.00012426345,0.96947014,0.000035646306,0.00006741875,0.0036120608,0.0005401618,0.011616822,0.008341249,0.0028149865,0.0033108776,0.000025065676],"about_ca_topic_score_codex":0.00050321734,"about_ca_topic_score_gemma":0.00044228934,"teacher_disagreement_score":0.00093088043,"about_ca_system_score_codex":0.00018761362,"about_ca_system_score_gemma":0.00005928561,"threshold_uncertainty_score":0.0031141043},"labels":[],"label_agreement":null},{"id":"W2155133805","doi":"10.1088/0004-637x/756/1/74","title":"A 2MASS ALL-SKY VIEW OF THE SAGITTARIUS DWARF GALAXY. VII. KINEMATICS OF THE MAIN BODY OF THE SAGITTARIUS dSph","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Milky Way; Sagittarius; Galactic Center; Stars; Proper motion; Velocity dispersion; Dwarf galaxy; Supermassive black hole; Giant star","score_opus":0.009138892082978436,"score_gpt":0.21943014793575774,"score_spread":0.2102912558527793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155133805","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08941947,0.0037150735,0.0069466042,0.0038553104,0.0017190534,0.00047307502,0.33551654,0.018648839,0.5397061],"genre_scores_gemma":[0.49626866,0.0035950246,0.03058914,0.0025509407,0.0012988475,0.0002444453,0.2822232,0.002128703,0.18110101],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9999443,0.0000067475535,0.0000023662164,0.000014489691,0.000015254417,0.000016845324],"domain_scores_gemma":[0.9998429,0.000008187101,0.000014959921,0.000014467233,0.00003882259,0.000080601225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000938997,0.00063191366,0.00028991696,0.0020107736,0.00044697316,0.00076449197,0.00040992486,0.0006052958,0.113377154],"category_scores_gemma":[0.00017460159,0.00019155527,0.00034521768,0.0017386144,0.00014385574,0.00053447275,0.0006334746,0.0007731296,0.036473114],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035383677,0.00018143335,0.044667903,0.00041009294,0.00016012613,0.0010623838,0.000642374,0.0009942283,0.032530382,0.004026826,0.8263887,0.08858173],"study_design_scores_gemma":[0.00011446194,0.00011061123,0.33263075,0.00013046096,0.000048616268,0.0006304867,0.0005975659,0.0014645203,0.0011136513,0.0015176599,0.6616197,0.000021538575],"about_ca_topic_score_codex":0.029854588,"about_ca_topic_score_gemma":0.051345788,"teacher_disagreement_score":0.113377154,"about_ca_system_score_codex":0.00036557327,"about_ca_system_score_gemma":0.00024883624,"threshold_uncertainty_score":0.37928438},"labels":[],"label_agreement":null},{"id":"W2155325347","doi":"10.1088/0004-637x/690/2/l122","title":"THE DETECTION OF INFRARED SiS BANDS IN SPECTRA OF S STARS","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Physics; Stars; Overtone; Rotational–vibrational spectroscopy; Astrophysics; Spectral line; Infrared; Context (archaeology); Line (geometry); Exoplanet; Astronomy; Infrared spectroscopy","score_opus":0.008847722312651062,"score_gpt":0.2162902898312344,"score_spread":0.20744256751858334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155325347","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960905,0.000079279176,0.00090695004,0.000023701134,0.0000043134078,0.000002719068,0.00011419828,0.00007562766,0.0027026597],"genre_scores_gemma":[0.9988834,0.000044321074,0.0006673622,0.000018645967,0.0000064456563,0.0000021574558,0.00016681691,0.0000070451297,0.0002039032],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999572,0.000003041162,0.0000022986915,0.000015372409,0.000010742003,0.000011332915],"domain_scores_gemma":[0.99973553,0.00005049741,0.000100076366,0.00002290315,0.000026874788,0.00006406805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008764722,0.00020465476,0.00011734018,0.00072265044,0.0002059485,0.00022977513,0.0001436715,0.0002534788,0.0011316685],"category_scores_gemma":[0.00028235934,0.00010348263,0.00012813226,0.0004078656,0.0003392617,0.00022235869,0.00024968895,0.00021425149,0.00022005176],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063388236,0.00011610896,0.28750116,0.00014698182,0.000053042288,0.0006841185,0.00059498806,0.001312629,0.68491566,0.0015913703,0.0006682186,0.021781776],"study_design_scores_gemma":[0.000018590505,0.00030718764,0.93161106,0.000015948368,0.000051483872,0.0013621005,0.0001803467,0.0033420082,0.060069602,0.0009596831,0.0020684376,0.000013574437],"about_ca_topic_score_codex":0.00024459796,"about_ca_topic_score_gemma":0.0003754488,"teacher_disagreement_score":0.0011316685,"about_ca_system_score_codex":0.00009521341,"about_ca_system_score_gemma":0.000044826138,"threshold_uncertainty_score":0.0037857294},"labels":[],"label_agreement":null},{"id":"W2155394969","doi":"10.1086/519154","title":"Identification of Very Red Counterparts of SiO Maser and OH/IR Objects in the GLIMPSE Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Maser; Line (geometry); Spectral line; Emission spectrum; Solar mass; Spectral resolution; High resolution","score_opus":0.011932027637023711,"score_gpt":0.25446744668297244,"score_spread":0.24253541904594872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155394969","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99956065,0.000037107213,0.00008644256,0.0000036576173,4.951818e-7,0.0000027415092,0.00004761145,0.0000054021557,0.0002559016],"genre_scores_gemma":[0.99880564,0.000082561324,0.00051873334,0.000016035341,0.000004979821,0.000006322097,0.0003488806,0.000004754163,0.00021199914],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998827,0.000010817635,0.000007464577,0.000028003793,0.00002691532,0.000044021413],"domain_scores_gemma":[0.9996044,0.00004205375,0.00015646785,0.000041233125,0.000033589367,0.00012226365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002123058,0.0002445961,0.00028511128,0.00125748,0.00035323715,0.00039549617,0.00017922542,0.00020855592,0.0008141793],"category_scores_gemma":[0.0004300046,0.00021492197,0.00014766715,0.00043336558,0.000366725,0.00028846174,0.00067379064,0.00017368651,0.0002182612],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017433627,0.00006156886,0.9493753,0.000021986829,0.00004108147,0.0008035866,0.00071352546,0.00008102983,0.040025678,0.00014672118,0.00017794181,0.008377272],"study_design_scores_gemma":[0.000003911476,0.000046877925,0.99799514,0.0000014348187,0.000008552726,0.00053217995,0.00014806373,0.000054722856,0.00084800407,0.000021970172,0.00033658647,0.0000024493972],"about_ca_topic_score_codex":0.0013277649,"about_ca_topic_score_gemma":0.0038873928,"teacher_disagreement_score":0.0013277649,"about_ca_system_score_codex":0.00012764824,"about_ca_system_score_gemma":0.00008869339,"threshold_uncertainty_score":0.0027236938},"labels":[],"label_agreement":null},{"id":"W2155615125","doi":"10.1088/0004-637x/700/2/1847","title":"A MULTI-IONIC KINEMATIC INVESTIGATION OF NGC 595, A GIANT EXTRAGALACTIC H II REGION IN M33","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Nebula; Line (geometry); Ionization; Orion Nebula; Galaxy; Interstellar medium; Photoionization; Stars; Forbidden mechanism; Molecular cloud; H II region; Plasma; Planetary nebula; Spectral line; Ion; Star formation; Emission spectrum; Astronomy","score_opus":0.019550150754378326,"score_gpt":0.249548298693477,"score_spread":0.22999814793909867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155615125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994221,0.00005662869,0.00009812154,0.000005130401,4.789725e-7,0.0000023076107,0.00007725718,0.0000035888904,0.00033445217],"genre_scores_gemma":[0.9990452,0.000052287265,0.00028698903,0.000009460035,0.0000018399481,0.000002137559,0.0003274643,0.0000020752636,0.0002725701],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999639,0.000002481149,0.0000018544265,0.000013051609,0.0000072105945,0.000011573466],"domain_scores_gemma":[0.9999474,0.000002716757,0.000018591425,0.0000034365564,0.000009040789,0.000018715005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005501662,0.00018818442,0.00008252935,0.0005819643,0.00023070241,0.00017974945,0.00014800871,0.00012315302,0.00045312542],"category_scores_gemma":[0.00008937235,0.00010541519,0.00013513675,0.0003308005,0.00009634465,0.00015952768,0.00022104957,0.00007863155,0.00014166521],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001426703,0.000053533615,0.66092473,0.000040177274,0.000025818354,0.0010628399,0.0005547743,0.0002890883,0.32605386,0.0002051087,0.00013165432,0.010515716],"study_design_scores_gemma":[0.0000015033845,0.0000306819,0.9974222,0.0000023371817,0.0000058261808,0.00023044895,0.00013579565,0.0002048731,0.0017008866,0.000017295064,0.00024682828,0.0000012405992],"about_ca_topic_score_codex":0.011320013,"about_ca_topic_score_gemma":0.018742627,"teacher_disagreement_score":0.011320013,"about_ca_system_score_codex":0.0002671311,"about_ca_system_score_gemma":0.00013726769,"threshold_uncertainty_score":0.022508264},"labels":[],"label_agreement":null},{"id":"W2155661075","doi":"10.1086/505525","title":"The Mass of the Central Black Hole in the Seyfert Galaxy NGC 4151","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Supermassive black hole; Galaxy; Solar mass; Black hole (networking); Ultraviolet; Active galactic nucleus","score_opus":0.007859716384835557,"score_gpt":0.20873164480775716,"score_spread":0.2008719284229216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155661075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999482,0.000055859728,0.000072426556,0.000008096045,0.0000010837947,9.836672e-7,0.0000542573,0.00001404574,0.00031137402],"genre_scores_gemma":[0.999485,0.000036120175,0.00013542788,0.000003120191,0.0000024868577,0.0000011840086,0.00016736066,0.0000022429228,0.0001671007],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999933,0.0000056234285,0.0000033150905,0.000028214892,0.000013899775,0.000015844938],"domain_scores_gemma":[0.9997639,0.000028889735,0.000113508795,0.000028500981,0.00002503295,0.000040214567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021369001,0.00032846807,0.00024860218,0.0011816161,0.0004004881,0.00059283513,0.0003013208,0.00029130784,0.0015214041],"category_scores_gemma":[0.0005469658,0.00013309142,0.00013676156,0.0003736307,0.00037036487,0.00047813586,0.00037903714,0.000158552,0.0003875718],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025972337,0.000028697214,0.93973505,0.000047265992,0.000080002756,0.0006426223,0.001308983,0.0014905821,0.036480628,0.0006458614,0.00039000568,0.018890621],"study_design_scores_gemma":[0.0000060719767,0.000043216936,0.9957436,0.000007334932,0.000019041321,0.00021999508,0.00020722617,0.0013287605,0.0018246829,0.0001563921,0.0004363437,0.0000073156157],"about_ca_topic_score_codex":0.005390204,"about_ca_topic_score_gemma":0.007883734,"teacher_disagreement_score":0.005390204,"about_ca_system_score_codex":0.0004284085,"about_ca_system_score_gemma":0.00008490491,"threshold_uncertainty_score":0.01071763},"labels":[],"label_agreement":null},{"id":"W2155730385","doi":"10.1088/0004-637x/752/1/1","title":"POSSIBLE DISINTEGRATING SHORT-PERIOD SUPER-MERCURY ORBITING KIC 12557548","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":224,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Bishop's University","funders":"Natural Sciences and Engineering Research Council of Canada; Yükseköğretim Kurulu; National Science Foundation","keywords":"Planet; Dwarf planet; Eclipse; Accretion (finance); Circumbinary planet; Giant planet; Binary star; Planetary system; Light curve; Stars","score_opus":0.015938767567735764,"score_gpt":0.24596092359014762,"score_spread":0.23002215602241186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155730385","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981377,0.00011163503,0.00020336271,0.000030009103,0.0000054914476,0.0000039007805,0.00004964477,0.000020816595,0.0014374722],"genre_scores_gemma":[0.9994523,0.000023446191,0.00019878714,0.000013371436,0.000003005681,0.0000019188976,0.0001046153,0.0000033039735,0.00019917978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999356,0.0000026643158,0.0000025964193,0.000018290046,0.000017872031,0.000022874423],"domain_scores_gemma":[0.9998617,0.000011860334,0.000057564594,0.000016328331,0.000015435326,0.000037074064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008095984,0.00026607953,0.00025699884,0.0005393966,0.00080747553,0.00039095012,0.00054128264,0.00052576046,0.0007300089],"category_scores_gemma":[0.00031275384,0.00016583341,0.00013711817,0.00048635065,0.00035167907,0.00025773278,0.00064208184,0.0002868798,0.00019868107],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007737466,0.00013699481,0.79562926,0.00019047801,0.00020566434,0.0184038,0.002647951,0.0026219555,0.1499909,0.0040039057,0.0017796577,0.023615696],"study_design_scores_gemma":[0.000047756315,0.00032847782,0.9585562,0.000036561083,0.000109102206,0.0053220163,0.0010351491,0.005983242,0.0155524835,0.0010427119,0.011933946,0.000052386662],"about_ca_topic_score_codex":0.006746728,"about_ca_topic_score_gemma":0.015013091,"teacher_disagreement_score":0.006746728,"about_ca_system_score_codex":0.00068478094,"about_ca_system_score_gemma":0.0001746975,"threshold_uncertainty_score":0.013414919},"labels":[],"label_agreement":null},{"id":"W2155808017","doi":"10.1086/516747","title":"On the Progenitors of Two Type II‐P Supernovae in the Virgo Cluster","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Red supergiant; Supernova; Physics; Supergiant; Virgo Cluster; Astrophysics; Advanced Camera for Surveys; Cluster (spacecraft); Astronomy; Hubble space telescope; Galaxy; Galaxy cluster; Stars; Computer science","score_opus":0.013489535115149009,"score_gpt":0.2560961342354179,"score_spread":0.24260659912026888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2155808017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983929,0.00014940798,0.00022144946,0.000012521007,0.0000022707225,0.0000054805023,0.000074375595,0.000013529428,0.0011280881],"genre_scores_gemma":[0.99827456,0.0001263618,0.0004638006,0.000018860661,0.000004303603,0.0000055458545,0.0006157855,0.0000067951696,0.00048401018],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991214,0.000009373039,0.0000051496067,0.000032492026,0.00002108952,0.000019715157],"domain_scores_gemma":[0.9997768,0.00002843494,0.000055652734,0.00003699918,0.000021836826,0.00008034159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021399831,0.00024146268,0.00014160715,0.0007849213,0.0004924738,0.0006076362,0.0002717732,0.00025462985,0.00051171373],"category_scores_gemma":[0.00042645438,0.00016262906,0.00013889362,0.00039847757,0.00023246596,0.0002045116,0.00088906754,0.00019711096,0.00028134816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061318994,0.00006643151,0.8717915,0.000047746307,0.00005041722,0.0030956243,0.0007308669,0.0015801525,0.10334704,0.0015122007,0.0003051192,0.016859632],"study_design_scores_gemma":[0.000010400125,0.00009276525,0.9843089,0.000016706737,0.000013858352,0.0023500584,0.0003186883,0.0020282017,0.007943625,0.0003684502,0.0025379858,0.000010310131],"about_ca_topic_score_codex":0.0028591512,"about_ca_topic_score_gemma":0.003312092,"teacher_disagreement_score":0.0028591512,"about_ca_system_score_codex":0.00033100208,"about_ca_system_score_gemma":0.000211788,"threshold_uncertainty_score":0.005685091},"labels":[],"label_agreement":null},{"id":"W2156052512","doi":"10.1088/0004-637x/791/1/67","title":"THE GREEN BANK NORTHERN CELESTIAL CAP PULSAR SURVEY. I. SURVEY DESCRIPTION, DATA ANALYSIS, AND INITIAL RESULTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":197,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Pulsar; Millisecond pulsar; Galactic plane; Sky; Green Bank Telescope; Radio telescope; Spectral index","score_opus":0.04315955892994607,"score_gpt":0.33693873674136826,"score_spread":0.2937791778114222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156052512","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17474873,0.004821528,0.0059775086,0.0025151013,0.0003814268,0.0026819075,0.7388838,0.0031695121,0.06682051],"genre_scores_gemma":[0.17420322,0.005294178,0.035621777,0.0031748717,0.00050250767,0.0044027427,0.7182697,0.001045416,0.05748555],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9991209,0.0001369413,0.00004784238,0.00019594583,0.000327496,0.00017080955],"domain_scores_gemma":[0.9972065,0.00015477237,0.00032622664,0.0003703338,0.0010765413,0.0008656458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015678582,0.00063805905,0.0005696008,0.0038541919,0.0011033418,0.0015193918,0.0011067885,0.00049765635,0.0094694905],"category_scores_gemma":[0.0017888799,0.00040545512,0.00023462567,0.0056275534,0.0003177874,0.0005503535,0.0014063315,0.00059887255,0.011143052],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064274576,0.00018904613,0.41208842,0.0004156808,0.00008916495,0.00052039296,0.00064339367,0.0007834029,0.003918474,0.0009852324,0.42886394,0.1508601],"study_design_scores_gemma":[0.00011239883,0.00010865731,0.7224698,0.00021315925,0.00003394683,0.00025996074,0.0003947546,0.0012579084,0.00087905943,0.0002549623,0.27398086,0.00003444027],"about_ca_topic_score_codex":0.19693016,"about_ca_topic_score_gemma":0.25637352,"teacher_disagreement_score":0.19693016,"about_ca_system_score_codex":0.0022841785,"about_ca_system_score_gemma":0.0040088403,"threshold_uncertainty_score":0.39156783},"labels":[],"label_agreement":null},{"id":"W2156085749","doi":"10.1088/0004-637x/785/1/12","title":"DYNAMICAL EVOLUTION OF VISCOUS DISKS AROUND BE STARS. II. POLARIMETRY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Observable; Physics; Polarimetry; Opacity; Stars; Polarization (electrochemistry); Radiative transfer; Astrophysics; Be star; Statistical physics; Scattering; Optics; Quantum mechanics","score_opus":0.007191532552997025,"score_gpt":0.2367179386300239,"score_spread":0.22952640607702687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156085749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872815,0.0003991304,0.007007222,0.000102703416,0.000010687916,0.000019649317,0.00027794365,0.000055126526,0.004845995],"genre_scores_gemma":[0.9965892,0.00028416506,0.0021194364,0.000020403455,0.000011592137,0.000007769215,0.00024542297,0.000016822733,0.0007050405],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999652,0.0000068307504,0.0000024287576,0.000009663193,0.0000075356343,0.00000846629],"domain_scores_gemma":[0.99988115,0.000028616596,0.00004482572,0.000013515074,0.000012208093,0.00001971351],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008101158,0.00016017014,0.000119967386,0.00040099217,0.00031070912,0.00067703583,0.0002369484,0.00023945753,0.00048317658],"category_scores_gemma":[0.00040846557,0.00012795058,0.0001427432,0.00023800443,0.00032875128,0.00032750214,0.0005453913,0.00023094803,0.00021199064],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032574014,0.00016051292,0.61697924,0.0001592164,0.00007810072,0.0011660826,0.0011980047,0.1697313,0.13746987,0.01966391,0.001219901,0.05184812],"study_design_scores_gemma":[0.00002480972,0.00021353415,0.56595826,0.000050275856,0.000035222605,0.000787366,0.0007322671,0.39331692,0.01956323,0.010732863,0.008508192,0.00007701171],"about_ca_topic_score_codex":0.0018659685,"about_ca_topic_score_gemma":0.0014462252,"teacher_disagreement_score":0.0018659685,"about_ca_system_score_codex":0.00033424833,"about_ca_system_score_gemma":0.00007610865,"threshold_uncertainty_score":0.00371027},"labels":[],"label_agreement":null},{"id":"W2156190218","doi":"10.1088/0004-637x/749/1/52","title":"THE McGill PLANAR HYDROGEN ATMOSPHERE CODE (McPHAC)","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Spectral line; Atmosphere (unit); Computational physics; Flux (metallurgy); Planar; Quantum mechanics; Computer science; Meteorology","score_opus":0.01266273725525223,"score_gpt":0.22436104711231397,"score_spread":0.21169830985706173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156190218","genre_codex":"methods","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.13791488,0.0015977263,0.36073926,0.0015032834,0.00081266084,0.0013579922,0.13725373,0.16293977,0.19588064],"genre_scores_gemma":[0.44705138,0.00086087076,0.3529558,0.0011673414,0.00016722786,0.00207784,0.08347113,0.036422033,0.07582631],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99957126,0.000071617906,0.000018047656,0.000055150515,0.00019599883,0.00008790095],"domain_scores_gemma":[0.9992756,0.00017961228,0.000053007687,0.0001526925,0.000263274,0.00007577275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000580493,0.00054159353,0.0004362737,0.00049076707,0.00052403787,0.0008716705,0.002689787,0.0006659288,0.038867284],"category_scores_gemma":[0.0021766392,0.00048514057,0.00058494863,0.0009358306,0.00032439688,0.0007284925,0.0009501142,0.0011175653,0.008304744],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013113124,0.00019638702,0.017209915,0.0010290818,0.0002060528,0.00054782175,0.00059815793,0.22227368,0.036498185,0.068504065,0.4403613,0.21126409],"study_design_scores_gemma":[0.0004791801,0.00014846389,0.007664916,0.00011818052,0.000057920803,0.00016730955,0.000120383695,0.47361317,0.03582879,0.008737228,0.47293997,0.00012449406],"about_ca_topic_score_codex":0.055790883,"about_ca_topic_score_gemma":0.05782014,"teacher_disagreement_score":0.055790883,"about_ca_system_score_codex":0.0019352575,"about_ca_system_score_gemma":0.0035654367,"threshold_uncertainty_score":0.13002408},"labels":[],"label_agreement":null},{"id":"W2156242403","doi":"10.1086/317089","title":"Membership and Multiplicity among Very Low Mass Stars and Brown Dwarfs in the Pleiades Cluster","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":142,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Pleiades; Brown dwarf; Physics; Stars; Astrophysics; Photometry (optics); Astronomy; Open cluster; Main sequence; Mass segregation","score_opus":0.00951903285891776,"score_gpt":0.21059853883543514,"score_spread":0.2010795059765174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156242403","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996767,0.00006556351,0.000030943527,0.000004753143,4.59804e-7,7.551641e-7,0.000034604545,0.000003431893,0.00018276306],"genre_scores_gemma":[0.9992447,0.000054667777,0.000116058625,0.0000049022133,0.0000033558954,0.0000022902248,0.00029384278,0.0000028217567,0.00027739353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975187,0.000034263445,0.000016364978,0.000074475916,0.00007123716,0.000051817144],"domain_scores_gemma":[0.99884903,0.00024148721,0.00038862473,0.0000935617,0.00009035111,0.00033692925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003253862,0.00020724307,0.00022956559,0.0019001692,0.0006599092,0.00073272537,0.00034173814,0.00024416833,0.0009397935],"category_scores_gemma":[0.0009810238,0.0001474277,0.000115014285,0.0008612248,0.00054088165,0.00027165894,0.000753248,0.00017849634,0.00023682034],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008886143,0.000018787412,0.9940069,0.0000124029975,0.000010866976,0.00008658956,0.0004402412,0.00011407303,0.0027047012,0.00008306551,0.00006905168,0.0023645072],"study_design_scores_gemma":[0.000001289669,0.000029945053,0.99917054,0.0000019263018,0.000007276626,0.00020981683,0.00011820355,0.000100054145,0.00018727871,0.000027281041,0.00014349095,0.0000029345858],"about_ca_topic_score_codex":0.004664567,"about_ca_topic_score_gemma":0.0074842637,"teacher_disagreement_score":0.004664567,"about_ca_system_score_codex":0.00030330836,"about_ca_system_score_gemma":0.00017696606,"threshold_uncertainty_score":0.00927484},"labels":[],"label_agreement":null},{"id":"W2156417646","doi":"10.1086/338079","title":"Are Stars with Planets Polluted?","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Metallicity; Planet; Stars; Stellar mass; Accretion (finance); Radial velocity; Stellar evolution; Stellar mass loss","score_opus":0.013937650964480656,"score_gpt":0.20095693998468095,"score_spread":0.1870192890202003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156417646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99539423,0.0007028456,0.0002468857,0.0006008252,0.000018028066,0.000005689209,0.0007381753,0.000022418171,0.002270939],"genre_scores_gemma":[0.9987191,0.00015821849,0.00006683031,0.00011360773,0.00003162626,0.0000023722998,0.00051604427,0.000006767947,0.0003853499],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989268,0.0001933366,0.00009215242,0.00037864843,0.0002088313,0.00020018421],"domain_scores_gemma":[0.99294853,0.0014363251,0.0039033426,0.0005142628,0.00054504303,0.0006525102],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007055266,0.00023115442,0.0005565189,0.0014181108,0.0009786343,0.0020444696,0.0005807583,0.0009275838,0.003819259],"category_scores_gemma":[0.0060469,0.00017764754,0.00031692965,0.0023076048,0.0010816905,0.0010320953,0.0012590734,0.00035743718,0.0012997345],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101951126,0.000011855272,0.99267536,0.000025385703,0.00008622974,0.00019231494,0.00051065435,0.00008127827,0.00080297765,0.00025731884,0.0002897462,0.0049649267],"study_design_scores_gemma":[0.0000071783065,0.000064768916,0.992273,0.000021260874,0.000060355094,0.0007267641,0.0013032021,0.00036784873,0.0007789036,0.0008128039,0.0035755513,0.000008425562],"about_ca_topic_score_codex":0.005992273,"about_ca_topic_score_gemma":0.0058281845,"teacher_disagreement_score":0.005992273,"about_ca_system_score_codex":0.000557423,"about_ca_system_score_gemma":0.0002737697,"threshold_uncertainty_score":0.012776673},"labels":[],"label_agreement":null},{"id":"W2156435016","doi":"10.1086/591313","title":"A Trio of New Local Group Galaxies with Extreme Properties","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":155,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Andromeda; Local Group; Milky Way; Dwarf galaxy problem; Dwarf galaxy; Dwarf spheroidal galaxy; Galaxy; Satellite galaxy","score_opus":0.0200020660533449,"score_gpt":0.18953027316137128,"score_spread":0.16952820710802638,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2156435016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9908728,0.0012969548,0.0012918469,0.00010410661,0.000023838023,0.000027514357,0.00041053415,0.00019871189,0.0057737916],"genre_scores_gemma":[0.99384034,0.0003791077,0.0015918269,0.0002285225,0.00006201364,0.000030739204,0.0013805204,0.00004721301,0.0024397771],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996438,0.000021630027,0.000015565505,0.00011469641,0.00010312134,0.00010116307],"domain_scores_gemma":[0.99891376,0.00013743724,0.00024215416,0.00024294663,0.00009863723,0.00036506538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034922527,0.0003780534,0.0004202512,0.0013618876,0.0006284365,0.0011022078,0.0006324222,0.0004016332,0.0039190915],"category_scores_gemma":[0.0007898031,0.00019804858,0.0004423403,0.0009829154,0.00066729257,0.0005490606,0.0011876741,0.00046637302,0.0015523295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028183206,0.00010669925,0.9251082,0.000112373185,0.000099207486,0.004632458,0.0016520799,0.00017694707,0.02242913,0.0011316267,0.0026892554,0.04158025],"study_design_scores_gemma":[0.000028032593,0.00021889023,0.95395356,0.000037339756,0.00006837808,0.021267997,0.0010384532,0.00029783294,0.002679932,0.0008561991,0.019519078,0.000034222365],"about_ca_topic_score_codex":0.0012479145,"about_ca_topic_score_gemma":0.0032097937,"teacher_disagreement_score":0.0039190915,"about_ca_system_score_codex":0.00034500676,"about_ca_system_score_gemma":0.00010852993,"threshold_uncertainty_score":0.013110697},"labels":[],"label_agreement":null},{"id":"W2157007497","doi":"10.1086/508645","title":"The Rotating Molecular Core and Precessing Outflow of the Young Stellar Object Barnard 1c","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Protostar; Astrophysics; Outflow; Torus; Young stellar object; Bipolar outflow; RADIUS; Jet (fluid); Molecular cloud; Star formation; Stars; Geometry","score_opus":0.0066793639140886605,"score_gpt":0.22615536378205636,"score_spread":0.2194759998679677,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157007497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99884194,0.000120709876,0.00007893106,0.000016627799,0.0000019816523,0.000003099177,0.000036453366,0.000012972696,0.0008872943],"genre_scores_gemma":[0.9989292,0.000056872927,0.00047225028,0.000027995264,0.000010128157,0.0000031971974,0.00022946604,0.0000070302435,0.00026370704],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999516,0.000002474627,8.6069514e-7,0.000016816282,0.000011841858,0.000016493103],"domain_scores_gemma":[0.9998652,0.0000105923855,0.00006298436,0.000009193359,0.000012553758,0.00003954009],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000070937705,0.0001566619,0.0002967706,0.0005069446,0.000619844,0.00050266815,0.00039541742,0.0004687202,0.00061234215],"category_scores_gemma":[0.00014547392,0.0001678647,0.00010002335,0.00025664576,0.00031218902,0.00022307283,0.000500219,0.00027866522,0.00030790185],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006475029,0.000240662,0.3521287,0.00014087769,0.000059397677,0.0035864604,0.0012754936,0.002496014,0.6147323,0.0018573108,0.0011044522,0.02173067],"study_design_scores_gemma":[0.000030435891,0.00019407665,0.97846586,0.0000126153445,0.00002408256,0.0014425021,0.0003143402,0.0060130088,0.009500924,0.00025071856,0.0037304638,0.000020943693],"about_ca_topic_score_codex":0.004715746,"about_ca_topic_score_gemma":0.005484968,"teacher_disagreement_score":0.004715746,"about_ca_system_score_codex":0.00053751864,"about_ca_system_score_gemma":0.00016083372,"threshold_uncertainty_score":0.0093765855},"labels":[],"label_agreement":null},{"id":"W2157056983","doi":"10.1086/516572","title":"Formation and Destruction of Small Binary Asteroids","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Asteroid; Physics; Primary (astronomy); Astronomy; Astrobiology; Planet; Astrophysics; Binary number; Contact binary; Binary star; Stars","score_opus":0.009462615753941993,"score_gpt":0.2066380277718541,"score_spread":0.1971754120179121,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157056983","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97049564,0.011845277,0.0073262854,0.00029554762,0.00006803289,0.00004033403,0.00013792128,0.00007130493,0.009719659],"genre_scores_gemma":[0.992357,0.0023875262,0.0025723705,0.000053819735,0.000026570688,0.000017510925,0.00014520109,0.000009657181,0.002430264],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998388,0.000013764658,0.000010745414,0.000077025165,0.000035515997,0.000024092502],"domain_scores_gemma":[0.99979633,0.000026740816,0.00007583407,0.000040943833,0.000018164039,0.000042115535],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030969564,0.00017019229,0.00026873816,0.00046657867,0.00052469637,0.0009616768,0.0004302797,0.00040806158,0.0008883973],"category_scores_gemma":[0.0005786152,0.0001732216,0.00018261196,0.00027574142,0.0006611421,0.00090335176,0.0009794739,0.00039032783,0.0003915439],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032442383,0.00014967402,0.18548113,0.0010797696,0.00010448422,0.002259856,0.0033915807,0.013647575,0.5010217,0.09212602,0.0019603248,0.19845353],"study_design_scores_gemma":[0.000051680243,0.00087277225,0.5159688,0.0002455619,0.000110942136,0.013277589,0.00273745,0.033661406,0.17489205,0.10699668,0.15108187,0.00010315069],"about_ca_topic_score_codex":0.0009550829,"about_ca_topic_score_gemma":0.00044697657,"teacher_disagreement_score":0.0009616768,"about_ca_system_score_codex":0.0007848409,"about_ca_system_score_gemma":0.00030540393,"threshold_uncertainty_score":0.005694449},"labels":[],"label_agreement":null},{"id":"W2157246770","doi":"10.1086/319105","title":"Fast Cosmic Microwave Background Analyses via Correlation Functions","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":148,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Monte Carlo method; Estimator; Algorithm; Multipole expansion; Cosmic background radiation; Covariance matrix; Weighting; Noise (video); Optics; Anisotropy; Statistics; Mathematics; Computer science","score_opus":0.021662816512947478,"score_gpt":0.2867558752166499,"score_spread":0.2650930587037024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157246770","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.02630062,0.0000725035,0.9706882,0.000040795123,0.000009831492,0.000012777529,0.00015493823,0.001740152,0.0009801502],"genre_scores_gemma":[0.4333444,0.00018093233,0.5635231,0.000051903477,0.00004540713,0.00008543632,0.0008435543,0.00063583435,0.0012893764],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99953604,0.000132247,0.000011378891,0.00006812213,0.00018784545,0.000064544234],"domain_scores_gemma":[0.99873203,0.00055317435,0.00019499971,0.00023570049,0.00023430178,0.0000497157],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010576803,0.00085556967,0.00055007706,0.0023342473,0.0004623946,0.00087085436,0.00088847056,0.00038875706,0.001310109],"category_scores_gemma":[0.0037763764,0.00050910626,0.00055453624,0.001576002,0.00048761835,0.001028373,0.0010735103,0.00067067036,0.00066104],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016737403,0.00009728555,0.014245705,0.00014833553,0.0002099629,0.0003087995,0.00023998992,0.47400358,0.043650284,0.09899621,0.004606168,0.36332637],"study_design_scores_gemma":[0.000011977125,0.000012465528,0.00307711,0.000008314894,0.000007523611,0.0000630879,0.000012413401,0.97019136,0.005548952,0.019234907,0.0018058129,0.000026046382],"about_ca_topic_score_codex":0.0049942974,"about_ca_topic_score_gemma":0.004896996,"teacher_disagreement_score":0.0049942974,"about_ca_system_score_codex":0.00053819845,"about_ca_system_score_gemma":0.0009980715,"threshold_uncertainty_score":0.009930491},"labels":[],"label_agreement":null},{"id":"W2157263660","doi":"10.1086/589323","title":"Determination of Effective Temperatures and Luminosities for Rotating Stars","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Stars; Astrophysics; Observer (physics); Rotation (mathematics); Luminosity; Stellar atmosphere; Plane (geometry); Stellar rotation; Effective temperature; Galaxy; Geometry","score_opus":0.008499895458341438,"score_gpt":0.230003209653126,"score_spread":0.22150331419478458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157263660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93840396,0.00013407855,0.05765917,0.000053730913,0.000010804416,0.000013408321,0.00023652472,0.00024819063,0.0032401138],"genre_scores_gemma":[0.99315333,0.00006989591,0.006078421,0.000007815114,0.0000054409065,0.000012900954,0.0003014099,0.00010361064,0.00026719662],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99973816,0.000049196693,0.000016544918,0.000078978,0.000073566254,0.000043525957],"domain_scores_gemma":[0.99921477,0.00022461003,0.00014098026,0.00017699876,0.00013266245,0.000109850414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005872286,0.00047085714,0.00046641016,0.00094582356,0.00049451535,0.001129493,0.000863528,0.00049819145,0.0006995471],"category_scores_gemma":[0.0033831033,0.0005160654,0.00069794996,0.0005703043,0.00056670606,0.00086497574,0.00065441435,0.00050921715,0.00032698832],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003131583,0.000064867396,0.16155107,0.00009467123,0.00014835075,0.00033494926,0.0006414008,0.69943416,0.06305107,0.052745387,0.00076750474,0.020853436],"study_design_scores_gemma":[0.00005305158,0.000066631575,0.04259783,0.000019432453,0.000059554277,0.00030587797,0.00013377369,0.9073431,0.0282289,0.018922955,0.0022045323,0.000064438376],"about_ca_topic_score_codex":0.0014356019,"about_ca_topic_score_gemma":0.0013148454,"teacher_disagreement_score":0.0014356019,"about_ca_system_score_codex":0.0012638512,"about_ca_system_score_gemma":0.00037908283,"threshold_uncertainty_score":0.009169996},"labels":[],"label_agreement":null},{"id":"W2157536284","doi":"10.1086/341196","title":"Gasdynamics in NGC 5248: Fueling a Circumnuclear Starburst Ring of Super–Star Clusters","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Spiral galaxy; Supernova; Bar (unit); Spiral (railway); Star formation; Galaxy; Star cluster; Star (game theory); Ring (chemistry); Astronomy","score_opus":0.012756361685247413,"score_gpt":0.2161995387520544,"score_spread":0.20344317706680698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157536284","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99928766,0.000022044811,0.00026515767,0.000014447264,9.249736e-7,0.0000013786379,0.000028312332,0.000014107884,0.00036595526],"genre_scores_gemma":[0.999655,0.000014440574,0.00020355204,0.0000019047975,0.0000013530333,0.0000015940683,0.000028551249,0.000002330675,0.0000912682],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996877,0.000006382376,0.0000013940728,0.000008399697,0.000004455969,0.00001061384],"domain_scores_gemma":[0.99987185,0.000028842971,0.000047174683,0.000019132704,0.0000098722,0.000023082675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008152919,0.00025337707,0.00023430109,0.00014709882,0.0002188831,0.0003360105,0.0005598406,0.0003109797,0.00079811254],"category_scores_gemma":[0.00035880142,0.00013496162,0.00021505274,0.00013052214,0.00027531848,0.00028106716,0.00026038222,0.00016920203,0.00010615804],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058648724,0.00024770445,0.46958804,0.00007981206,0.00010253966,0.0018084126,0.0006184871,0.46779162,0.045874827,0.0039568925,0.0010629953,0.008282284],"study_design_scores_gemma":[0.00010547153,0.0001585659,0.160157,0.0000060728426,0.00004195988,0.00031425676,0.00014040298,0.8344458,0.0029239438,0.000925938,0.00075899577,0.000021539936],"about_ca_topic_score_codex":0.028601266,"about_ca_topic_score_gemma":0.017088138,"teacher_disagreement_score":0.028601266,"about_ca_system_score_codex":0.0005128185,"about_ca_system_score_gemma":0.00017530541,"threshold_uncertainty_score":0.056869566},"labels":[],"label_agreement":null},{"id":"W2157545454","doi":"10.1088/0004-637x/774/1/48","title":"INTO THE LAIR: GRAVITATIONAL-WAVE SIGNATURES OF DARK MATTER","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":228,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Fundação para a Ciência e a Tecnologia; Institut Périmètre de physique théorique; Ministero dello Sviluppo Economico; Kindai University; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; FP7 People: Marie-Curie Actions; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Industry Canada; Partnership for Advanced Computing in Europe AISBL; San Diego Supercomputer Center; European Commission; National Science Foundation; Government of Canada; CERN","keywords":"Physics; Dark matter; Astronomy; Gravitational wave; Astrophysics","score_opus":0.005481447605790561,"score_gpt":0.22834172921619442,"score_spread":0.22286028161040386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157545454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9415109,0.003018077,0.027978802,0.0015370497,0.00009327265,0.000024215811,0.00015188975,0.0005284264,0.025157321],"genre_scores_gemma":[0.9936132,0.00036111812,0.0034656315,0.00016932047,0.00007913158,0.000004784065,0.000066479384,0.00006297096,0.0021774317],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999453,0.000018498748,0.0000017123749,0.00001222766,0.000011036418,0.00001119193],"domain_scores_gemma":[0.9998745,0.000026396176,0.00003580494,0.000019475501,0.000011550072,0.000032294058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024580618,0.00027247317,0.00023882616,0.00042423359,0.00033296086,0.000903733,0.0004067536,0.0004018038,0.0017342921],"category_scores_gemma":[0.00048659852,0.000121081495,0.00020984508,0.0002521795,0.00066417287,0.00075375853,0.0007348547,0.0005816236,0.0002536316],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012943507,0.00029644035,0.10223197,0.00056115026,0.00024029113,0.0042691566,0.0048358585,0.03067722,0.21901828,0.5265199,0.0077036256,0.10235171],"study_design_scores_gemma":[0.00013023197,0.0005883547,0.17916635,0.00013320621,0.000100813944,0.0023086239,0.0013984588,0.4286322,0.01601762,0.34690073,0.024486229,0.00013724288],"about_ca_topic_score_codex":0.00067623844,"about_ca_topic_score_gemma":0.0005710827,"teacher_disagreement_score":0.0017342921,"about_ca_system_score_codex":0.0002571633,"about_ca_system_score_gemma":0.000096862736,"threshold_uncertainty_score":0.0058017373},"labels":[],"label_agreement":null},{"id":"W2157672340","doi":"10.1086/527355","title":"Millihertz Oscillation Frequency Drift Predicts the Occurrence of Type I X-Ray Bursts","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Neutron star; Astrophysics; Oscillation (cell signaling); Thermonuclear fusion; Observable; Low frequency; Astronomy; Plasma; Nuclear physics; Chemistry; Quantum mechanics","score_opus":0.02108891960317785,"score_gpt":0.23604114863027356,"score_spread":0.2149522290270957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157672340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99842286,0.0000726801,0.0009113963,0.000016154037,0.000003273349,0.0000027682856,0.00005809985,0.000018460316,0.00049419905],"genre_scores_gemma":[0.99965656,0.000023893566,0.0001936231,0.0000030043518,0.000004049797,0.0000023229231,0.00007247307,0.000002440728,0.00004162759],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999498,0.0000068655463,0.0000056553135,0.000015828291,0.000009742305,0.000012060054],"domain_scores_gemma":[0.99851996,0.000666548,0.0005497854,0.000089177076,0.00007299156,0.00010159005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028565055,0.00020797708,0.00020394726,0.0005528416,0.00017414238,0.00036208867,0.000188854,0.00028294223,0.0007989888],"category_scores_gemma":[0.0019457189,0.00015605718,0.00012304902,0.00023335824,0.00019714065,0.00028932357,0.00027494758,0.00029179401,0.00024265886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027293098,0.00003837499,0.9677274,0.000021185853,0.000029390818,0.00014365755,0.000085963155,0.009962823,0.015195027,0.00044008956,0.00013139406,0.005951721],"study_design_scores_gemma":[0.000012603856,0.00008022023,0.94097126,0.000007462027,0.000018479584,0.00020594195,0.00004721421,0.05441862,0.0036888141,0.00031182126,0.00022654653,0.000010974465],"about_ca_topic_score_codex":0.0010665801,"about_ca_topic_score_gemma":0.0009423968,"teacher_disagreement_score":0.0010665801,"about_ca_system_score_codex":0.0002169243,"about_ca_system_score_gemma":0.00007938233,"threshold_uncertainty_score":0.0026729107},"labels":[],"label_agreement":null},{"id":"W2157719001","doi":"10.1088/0004-637x/766/2/104","title":"THE RISE OF AN IONIZED WIND IN THE NARROW-LINE SEYFERT 1 GALAXY Mrk 335 OBSERVED BY<i>XMM-NEWTON</i>AND<i>HST</i>","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Photoionization; Ionization; Flux (metallurgy); Galaxy; Spectral line; Absorption (acoustics)","score_opus":0.014314183411911473,"score_gpt":0.22583829136867667,"score_spread":0.21152410795676518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157719001","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99955016,0.000076013464,0.00006989919,0.000013318158,0.0000017394412,0.00000204438,0.00006744049,0.000015157078,0.00020416094],"genre_scores_gemma":[0.99943954,0.00004819556,0.00025327847,0.00001057966,0.0000071764102,0.0000023212851,0.0001580962,0.0000026803193,0.0000782001],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999523,0.0000038169346,0.0000025880768,0.000013710394,0.000011625822,0.000015892494],"domain_scores_gemma":[0.99979705,0.0000116533865,0.00012224092,0.000015051507,0.000010826119,0.000043159063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000864266,0.0002197113,0.00014261995,0.00053798716,0.00020597107,0.0003963369,0.00020670235,0.00033715766,0.0005697566],"category_scores_gemma":[0.00023885602,0.00013596799,0.00017665804,0.00032176892,0.0002206459,0.00022899218,0.00031801715,0.00025939607,0.00018345455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059788197,0.000109060726,0.7172748,0.00012335427,0.00011340045,0.004900617,0.0007702866,0.0011274853,0.26117265,0.000400618,0.0006008955,0.012808975],"study_design_scores_gemma":[0.000008334255,0.00015528715,0.9955844,0.000006221541,0.0000272483,0.0007638616,0.00008742103,0.00073709956,0.0020866462,0.00004987665,0.00048648572,0.000006961957],"about_ca_topic_score_codex":0.001670484,"about_ca_topic_score_gemma":0.0023943242,"teacher_disagreement_score":0.001670484,"about_ca_system_score_codex":0.00016461089,"about_ca_system_score_gemma":0.00006283255,"threshold_uncertainty_score":0.0033215284},"labels":[],"label_agreement":null},{"id":"W2157847746","doi":"10.1088/0004-637x/701/2/1958","title":"CONSTRAINTS ON THE HIGH-ℓ POWER SPECTRUM OF MILLIMETER-WAVE ANISOTROPIES FROM APEX-SZ","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Lawrence Berkeley National Laboratory; Nuclear Physics; Natural Sciences and Engineering Research Council of Canada; McGill University; U.S. Department of Energy; Office of Science; National Science Foundation","keywords":"Physics; Cosmic microwave background; Astrophysics; Amplitude; Galaxy; Millimeter; Population; Spectral density; Anisotropy; Point source; Sky; Optics; Telecommunications","score_opus":0.008650648161582206,"score_gpt":0.19646629263341814,"score_spread":0.18781564447183594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157847746","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96359444,0.00047086485,0.014832693,0.00028020312,0.000028642107,0.000019333589,0.003049226,0.000546997,0.017177531],"genre_scores_gemma":[0.99175256,0.00015795753,0.004369916,0.00004977161,0.00005515839,0.000015813062,0.0030596056,0.00009378071,0.00044536212],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959975,0.000030790932,0.0000147855335,0.000099578036,0.00016866626,0.00008649493],"domain_scores_gemma":[0.9988644,0.00033969624,0.00023246557,0.00023824403,0.00015674211,0.00016848385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007017075,0.0007291749,0.00043238245,0.0008843139,0.00027195254,0.001084155,0.0006596872,0.000330092,0.0027763878],"category_scores_gemma":[0.0016473172,0.0005013695,0.00041211772,0.0007421011,0.00030803395,0.0006287031,0.0009317674,0.00073504413,0.0009398136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011205708,0.000097736105,0.6211787,0.00028963276,0.00035805657,0.00077790854,0.00061277143,0.01759521,0.25707996,0.015409517,0.0048534693,0.08062641],"study_design_scores_gemma":[0.00009516523,0.000080313366,0.9245415,0.000033161534,0.000113555034,0.00034478054,0.0000793941,0.029951029,0.03212896,0.0039399946,0.008609381,0.00008288396],"about_ca_topic_score_codex":0.001305281,"about_ca_topic_score_gemma":0.002567167,"teacher_disagreement_score":0.0027763878,"about_ca_system_score_codex":0.0005560269,"about_ca_system_score_gemma":0.00023358285,"threshold_uncertainty_score":0.009287953},"labels":[],"label_agreement":null},{"id":"W2157873409","doi":"10.1086/339241","title":"Radio Galaxies at<i>z</i>= 1.1 to 3.8: Adaptive Optics Imaging and Archival<i>Hubble Space Telescope</i>Data","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Redshift; Astrophysics; Astronomy; Hubble Deep Field South; Hubble Deep Field; Galaxy; Hubble Ultra-Deep Field; Radio galaxy; Hubble space telescope; Wide Field Camera 3; Quasar","score_opus":0.014513471524518403,"score_gpt":0.21371587819312335,"score_spread":0.19920240666860495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157873409","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97968113,0.0002027605,0.0008649935,0.00007213079,0.000008043958,0.000053852425,0.016094333,0.0001887412,0.0028340116],"genre_scores_gemma":[0.92428446,0.00030879572,0.012326565,0.00011581983,0.00006141104,0.000090320566,0.059711803,0.00007621293,0.003024691],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997545,0.000015126773,0.000016518718,0.00005457031,0.00008276808,0.00007651818],"domain_scores_gemma":[0.9987795,0.000047869697,0.00030793506,0.00023433015,0.00031657552,0.00031382116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050947035,0.00029788405,0.0002391997,0.0020213905,0.0004805835,0.0005150484,0.0005746679,0.00022320624,0.0017662622],"category_scores_gemma":[0.00052748347,0.0001845678,0.00028425767,0.0015257797,0.00020310952,0.00037091327,0.0004916757,0.00039269167,0.00090851524],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043729754,0.00024101959,0.89301103,0.00010083764,0.00011604859,0.00033032597,0.0010042685,0.0008089958,0.043948743,0.0005601912,0.007427236,0.052013934],"study_design_scores_gemma":[0.0000119243,0.000021986554,0.99391806,0.0000039010956,0.000018162562,0.00007978947,0.00005395279,0.00021302774,0.0021914083,0.000056711127,0.0034260144,0.000005106762],"about_ca_topic_score_codex":0.027815789,"about_ca_topic_score_gemma":0.06346948,"teacher_disagreement_score":0.027815789,"about_ca_system_score_codex":0.0005486492,"about_ca_system_score_gemma":0.0004542828,"threshold_uncertainty_score":0.055307746},"labels":[],"label_agreement":null},{"id":"W2157910579","doi":"10.1086/522193","title":"Scaling Relations of Spiral Galaxies","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":250,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Surface brightness; Luminosity; Spiral galaxy; Galaxy; Brightness; Velocity dispersion; Scaling; Fundamental plane (elliptical galaxies); Elliptical galaxy; Astronomy; Lenticular galaxy; Geometry; Mathematics","score_opus":0.00876395364213504,"score_gpt":0.22524965594539825,"score_spread":0.21648570230326322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2157910579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99298793,0.0003703759,0.0023346967,0.00004997267,0.0000027881633,0.000010077918,0.00085490756,0.00010196787,0.0032871729],"genre_scores_gemma":[0.99767977,0.00011537701,0.00086333044,0.0000058445494,0.000006295878,0.000012286698,0.0011062607,0.00001484462,0.00019605881],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997049,0.00005924715,0.000023155406,0.00011226697,0.000060576025,0.000039869858],"domain_scores_gemma":[0.99755055,0.0008341481,0.00063204253,0.000485566,0.00026342703,0.00023427226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040956086,0.00030388148,0.00024762802,0.0032926085,0.0002949782,0.0007770498,0.0002461364,0.00017430667,0.0021708452],"category_scores_gemma":[0.0053949277,0.00016261247,0.0004203251,0.0020602136,0.00057999574,0.00059370534,0.00045454723,0.00024909523,0.00043782702],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000058076967,0.000028894463,0.93106645,0.00004794574,0.0001024296,0.00016873202,0.00095772033,0.009465122,0.0036829566,0.00939174,0.0009677944,0.044062093],"study_design_scores_gemma":[0.000014891055,0.000070297545,0.95578146,0.00002853418,0.000030839685,0.00044386642,0.0003887108,0.018991591,0.0005180216,0.018663106,0.005041489,0.000027141123],"about_ca_topic_score_codex":0.0051999395,"about_ca_topic_score_gemma":0.0049051982,"teacher_disagreement_score":0.0051999395,"about_ca_system_score_codex":0.0007566152,"about_ca_system_score_gemma":0.0001918331,"threshold_uncertainty_score":0.01033932},"labels":[],"label_agreement":null},{"id":"W2158023309","doi":"10.1088/0004-637x/773/1/57","title":"TESTING THE NO-HAIR THEOREM WITH OBSERVATIONS IN THE ELECTROMAGNETIC SPECTRUM. IV. RELATIVISTICALLY BROADENED IRON LINES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Multipole expansion; Spin (aerodynamics); Black hole (networking); Kerr metric; Metric (unit); Line (geometry); Computational physics; Rotating black hole; Astrophysics; Spins; Accretion (finance); Quantum mechanics; Geometry; Condensed matter physics; Schwarzschild radius","score_opus":0.015987618729850227,"score_gpt":0.21206224594949818,"score_spread":0.19607462721964797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158023309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98287326,0.0001373774,0.014856178,0.00006345034,0.000011437328,0.000014458966,0.000096466254,0.0000743735,0.0018728825],"genre_scores_gemma":[0.996007,0.000020164714,0.0037928075,0.000011611724,0.0000047635017,0.0000036700756,0.000062805506,0.000011163627,0.00008591849],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994412,0.00017344319,0.00002118711,0.00013980347,0.00014427818,0.000080071644],"domain_scores_gemma":[0.99745005,0.0009388601,0.000751203,0.0005030882,0.00015825815,0.00019846724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017451714,0.00039743126,0.00021451291,0.0006700631,0.0002363115,0.0006578473,0.00062661176,0.00066447584,0.00081440265],"category_scores_gemma":[0.005840047,0.00022843022,0.00038627142,0.0004227839,0.0008869894,0.0011178241,0.0010508057,0.0005137765,0.00026946297],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015964868,0.00039220048,0.7073752,0.00018554262,0.00036043956,0.0010710713,0.00047359103,0.083524875,0.10946294,0.03921167,0.00071270316,0.055633236],"study_design_scores_gemma":[0.00016986002,0.0006498735,0.49043483,0.000067758585,0.00009768847,0.0007317509,0.00034919585,0.42086685,0.047084115,0.037465967,0.0020032057,0.00007888542],"about_ca_topic_score_codex":0.0009610077,"about_ca_topic_score_gemma":0.0007937495,"teacher_disagreement_score":0.0017451714,"about_ca_system_score_codex":0.00034301833,"about_ca_system_score_gemma":0.00017060968,"threshold_uncertainty_score":0.009229422},"labels":[],"label_agreement":null},{"id":"W2158077998","doi":"10.1088/0004-637x/766/1/56","title":"REPRODUCING THE STELLAR MASS/HALO MASS RELATION IN SIMULATED ΛCDM GALAXIES: THEORY VERSUS OBSERVATIONAL ESTIMATES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":185,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Halo; Galaxy; Stellar mass; Supernova; Star formation; Baryon; Astronomy; Solar mass; Galaxy formation and evolution","score_opus":0.018012976419429505,"score_gpt":0.2319331992663796,"score_spread":0.2139202228469501,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158077998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99497765,0.000033167416,0.003830058,0.00005659012,0.0000034416519,0.00001065652,0.00031007366,0.00007848081,0.00069993024],"genre_scores_gemma":[0.9975988,0.000020513668,0.002005469,0.000016858996,0.0000034616353,0.00001147264,0.0002537083,0.000014899309,0.000074847914],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979705,0.00007195616,0.000011610546,0.000053925425,0.00003595272,0.000029510453],"domain_scores_gemma":[0.9973348,0.0014606504,0.00040458786,0.00034733993,0.00030670068,0.0001458369],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013731382,0.00039956337,0.0002910269,0.0005397124,0.00029449095,0.0005851045,0.0012405744,0.0006388939,0.0006437611],"category_scores_gemma":[0.0061347857,0.0002888958,0.00040540117,0.00040115163,0.00047546576,0.0005972192,0.00039257004,0.00035017176,0.00013123099],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012879378,0.000088836474,0.1873699,0.000040909363,0.0000807471,0.00007374916,0.00012249534,0.80412453,0.0022788686,0.00159177,0.00024556342,0.0038538312],"study_design_scores_gemma":[0.000041791485,0.000056702636,0.022463921,0.000009804482,0.00001756271,0.000028311235,0.000040032264,0.97525746,0.001231346,0.00067099597,0.00016986176,0.000012170068],"about_ca_topic_score_codex":0.015287478,"about_ca_topic_score_gemma":0.009602271,"teacher_disagreement_score":0.015287478,"about_ca_system_score_codex":0.001174759,"about_ca_system_score_gemma":0.00041640594,"threshold_uncertainty_score":0.030396998},"labels":[],"label_agreement":null},{"id":"W2158150762","doi":"10.1086/429366","title":"Spectroscopic Constants, Abundances, and Opacities of the TiH Molecule","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Subdwarf; Opacity; Spectral line; Line (geometry); Molecule; Titanium; Infrared; Absorption spectroscopy","score_opus":0.006647235870687686,"score_gpt":0.22426357415557754,"score_spread":0.21761633828488985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158150762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99413574,0.00036895197,0.002085583,0.0000397375,0.000007569287,0.000006866904,0.00026288602,0.000041866304,0.00305067],"genre_scores_gemma":[0.9978891,0.00015944865,0.001303805,0.0000080089185,0.000010447692,0.0000036603428,0.00021409069,0.000005106923,0.00040635274],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99996316,0.0000032132905,0.0000012235794,0.000011085943,0.000011975644,0.000009447016],"domain_scores_gemma":[0.9998516,0.000036516114,0.000052881263,0.000023258273,0.000018201252,0.000017462255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014618268,0.00012724308,0.00006935762,0.00097330817,0.00030219622,0.00024415646,0.0003138659,0.00018554286,0.0020823642],"category_scores_gemma":[0.00048391617,0.000099291625,0.00011612933,0.00034262956,0.00028478418,0.0004248692,0.0001966983,0.00022264275,0.00032639096],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030389358,0.00015277132,0.5459379,0.0002234885,0.00010343395,0.00036658943,0.00089397276,0.016469896,0.35784397,0.012975517,0.0010970454,0.06363152],"study_design_scores_gemma":[0.000090377536,0.00046337748,0.72646034,0.00003897085,0.00010763317,0.0010997445,0.00084454584,0.077157326,0.169753,0.008364097,0.015537048,0.00008360533],"about_ca_topic_score_codex":0.0015415663,"about_ca_topic_score_gemma":0.0013065919,"teacher_disagreement_score":0.0020823642,"about_ca_system_score_codex":0.00054580416,"about_ca_system_score_gemma":0.00011396459,"threshold_uncertainty_score":0.0069662333},"labels":[],"label_agreement":null},{"id":"W2158379565","doi":"10.1086/505559","title":"A Measurement of the Angular Power Spectrum of the CMB Temperature Anisotropy from the 2003 Flight of BOOMERANG","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":239,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Multipole expansion; Physics; Planck; Astrophysics; Anisotropy; Sky; Spectral density; Polarization (electrochemistry); Computational physics; Astronomy; Optics; Statistics","score_opus":0.003523041019861912,"score_gpt":0.19087109303954694,"score_spread":0.18734805201968502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158379565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99646854,0.00014244812,0.00065352384,0.000045108718,0.0000093002445,0.000015007336,0.0012311139,0.00004712975,0.0013877989],"genre_scores_gemma":[0.99533975,0.00012333225,0.00141448,0.00002589804,0.000017681185,0.0000142346125,0.0027288615,0.000020103564,0.00031565587],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998443,0.000015217033,0.00000358117,0.000043125063,0.000045577646,0.000048173068],"domain_scores_gemma":[0.99962103,0.000028712526,0.00013751959,0.000050384937,0.00006720167,0.00009512405],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020445329,0.00041796712,0.00020565375,0.0011957843,0.0004975859,0.00037617626,0.00022589353,0.0002698566,0.00055116747],"category_scores_gemma":[0.0004420109,0.00019120747,0.00018834058,0.0011010471,0.00036305474,0.00018177566,0.00036135642,0.00047570872,0.00025531295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009493515,0.0002178367,0.8577762,0.00009975755,0.00026879238,0.00068726216,0.001805011,0.0015583216,0.097636744,0.0004178153,0.002419141,0.036163688],"study_design_scores_gemma":[0.00000872833,0.000052189796,0.99536335,0.0000036400118,0.000017106016,0.0001502687,0.0000502922,0.0004666299,0.0023283781,0.000033014057,0.0015157956,0.000010503863],"about_ca_topic_score_codex":0.02834959,"about_ca_topic_score_gemma":0.07516593,"teacher_disagreement_score":0.02834959,"about_ca_system_score_codex":0.0005909991,"about_ca_system_score_gemma":0.00024076016,"threshold_uncertainty_score":0.056369126},"labels":[],"label_agreement":null},{"id":"W2158598196","doi":"10.1086/320261","title":"The Effect of Radiative Cooling on Scaling Laws of X-Ray Groups and Clusters","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Radiative cooling; Radiative transfer; Scaling; Cosmology; Cluster (spacecraft); Dark matter; Intracluster medium","score_opus":0.004554605075676001,"score_gpt":0.21020392045822955,"score_spread":0.20564931538255354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158598196","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99752873,0.00006380542,0.00081318367,0.00010725501,0.000007469843,0.000010386925,0.00007843345,0.000042713902,0.0013480731],"genre_scores_gemma":[0.9981495,0.00004787296,0.0012945228,0.000029585202,0.0000068240597,0.000017187682,0.00014308249,0.000055233228,0.00025615498],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9995912,0.00019013422,0.000016766991,0.000060797673,0.0000528562,0.0000881406],"domain_scores_gemma":[0.9969104,0.0017569086,0.00033962715,0.00039234676,0.00024912145,0.0003516011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012874925,0.0005048826,0.0004485415,0.0004835086,0.0006783246,0.0008329437,0.0010387369,0.0004322883,0.0012981126],"category_scores_gemma":[0.009672902,0.0003415097,0.0006521776,0.00043651203,0.0009988163,0.00085824524,0.00073748274,0.00082415814,0.0001189605],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003805256,0.00015802195,0.06390246,0.000058179066,0.00016786861,0.00020034953,0.00034383542,0.9160573,0.0075842836,0.00634021,0.00062808045,0.0041789236],"study_design_scores_gemma":[0.00012903896,0.00023109799,0.01800255,0.000014983171,0.000055038192,0.00004568025,0.00015594786,0.9749165,0.0036717332,0.002148088,0.00059738633,0.000031820142],"about_ca_topic_score_codex":0.012856822,"about_ca_topic_score_gemma":0.008831589,"teacher_disagreement_score":0.012856822,"about_ca_system_score_codex":0.00086504663,"about_ca_system_score_gemma":0.00069678226,"threshold_uncertainty_score":0.025563955},"labels":[],"label_agreement":null},{"id":"W2158677910","doi":"10.1086/340586","title":"Electrodynamics of Magnetars: Implications for the Persistent X‐Ray Emission and Spin‐down of the Soft Gamma Repeaters and Anomalous X‐Ray Pulsars","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":649,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Magnetar; Neutron star; Magnetosphere; Astrophysics; Magnetic dipole; Pulsar; Electron; Magnetic field; Dipole; Atomic physics; Nuclear physics","score_opus":0.01181059432343133,"score_gpt":0.27333603702883785,"score_spread":0.2615254427054065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158677910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97246504,0.001088309,0.013680766,0.0011295974,0.000059834503,0.00001093952,0.00004428744,0.00004549938,0.011475661],"genre_scores_gemma":[0.99656564,0.00032450352,0.0015832161,0.000072607894,0.000060091043,0.000010489767,0.000017145034,0.000010764467,0.0013554718],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999654,0.000008142504,0.0000018920942,0.000006312499,0.000008542643,0.000009568338],"domain_scores_gemma":[0.9999107,0.000026464384,0.000028134891,0.000010623319,0.000009103963,0.000014944608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001252786,0.00018636219,0.00014885879,0.00018400533,0.00032260345,0.000635352,0.0002865564,0.00037065806,0.0007777302],"category_scores_gemma":[0.00027857197,0.00008380642,0.0002438233,0.00012240944,0.0007027153,0.0005798189,0.00052447664,0.00019562973,0.000101751524],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002416453,0.00011354921,0.06505555,0.00009257114,0.00008025756,0.0016826269,0.0012056954,0.08671668,0.10923146,0.7006642,0.0019585195,0.0329572],"study_design_scores_gemma":[0.0001315293,0.00059028406,0.17046487,0.000044474637,0.000048785176,0.003310589,0.0014470121,0.42838696,0.019882604,0.35674313,0.018857855,0.00009193642],"about_ca_topic_score_codex":0.00056128664,"about_ca_topic_score_gemma":0.00045194844,"teacher_disagreement_score":0.0007777302,"about_ca_system_score_codex":0.00028457926,"about_ca_system_score_gemma":0.00011447814,"threshold_uncertainty_score":0.0026017427},"labels":[],"label_agreement":null},{"id":"W2158681003","doi":"10.1088/0004-637x/808/2/110","title":"<i>VERITAS</i>DETECTION OF<i>γ</i>-RAY FLARING ACTIVITY FROM THE BL LAC OBJECT 1ES 1727+502 DURING BRIGHT MOONLIGHT OBSERVATIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"BL Lac object; Blazar; Extragalactic background light; Crab Nebula; Cherenkov radiation; Telescope; Fermi Gamma-ray Space Telescope; Spectral energy distribution","score_opus":0.01778133386635836,"score_gpt":0.2131422452567811,"score_spread":0.19536091139042275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158681003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9869463,0.0008453648,0.00082236214,0.00012216762,0.000048818158,0.000031207765,0.0021628414,0.00061329606,0.00840766],"genre_scores_gemma":[0.9911481,0.00019894517,0.0022201433,0.0001292226,0.00008270703,0.000023996763,0.004797316,0.00007919056,0.0013203194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970883,0.000013319727,0.000011678346,0.000087109365,0.000105969586,0.000073045376],"domain_scores_gemma":[0.99957246,0.000027125765,0.00017475829,0.0000609054,0.00007012014,0.000094631556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033705655,0.0003686775,0.00032517314,0.0012947934,0.0004416197,0.00089967187,0.000528362,0.0005306208,0.0018436067],"category_scores_gemma":[0.00039373807,0.00023903645,0.0003377472,0.0006825156,0.00032596992,0.0002700172,0.00073458406,0.00046237386,0.0004899886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014133655,0.00014108908,0.4895147,0.00054010516,0.00040636657,0.0038701864,0.0011623554,0.00089567614,0.4371588,0.0010288935,0.009777286,0.054091193],"study_design_scores_gemma":[0.000040060688,0.00018533981,0.96044904,0.000031485462,0.00009322324,0.0019310099,0.00013555677,0.0007754484,0.025660396,0.00009750399,0.010571978,0.000028985305],"about_ca_topic_score_codex":0.004701437,"about_ca_topic_score_gemma":0.012131535,"teacher_disagreement_score":0.004701437,"about_ca_system_score_codex":0.00051105133,"about_ca_system_score_gemma":0.0002229176,"threshold_uncertainty_score":0.009348154},"labels":[],"label_agreement":null},{"id":"W2158780928","doi":"10.1088/0004-637x/743/1/62","title":"VERITAS OBSERVATIONS OF GAMMA-RAY BURSTS DETECTED BY<i>SWIFT</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Gamma-ray burst; Astrophysics; Fermi Gamma-ray Space Telescope; Telescope; Context (archaeology); Swift; Gamma ray; On board; Astronomy","score_opus":0.023718112579534812,"score_gpt":0.21936332564581523,"score_spread":0.1956452130662804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158780928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99593323,0.000078158555,0.00020684209,0.000013725636,0.000008459529,0.00000927897,0.0026390357,0.000055404278,0.0010559207],"genre_scores_gemma":[0.98810136,0.00008354184,0.0013086201,0.000019308229,0.000018294948,0.00001324201,0.009779241,0.000028175815,0.00064825616],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979573,0.000014010236,0.000019339637,0.000053697655,0.000055951918,0.00006134553],"domain_scores_gemma":[0.9989034,0.00013655575,0.00055509043,0.00013711087,0.0001399336,0.0001279243],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034579623,0.00023733775,0.0002464569,0.0010924804,0.00032767458,0.00049591187,0.00044362806,0.00027850826,0.0014271459],"category_scores_gemma":[0.00062872405,0.00021696524,0.00028167292,0.0006514125,0.00019337518,0.00026590735,0.0005492734,0.00037722307,0.00026594743],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001345256,0.00021760914,0.9076761,0.00011275243,0.00028452993,0.00077347347,0.0004918558,0.0025571843,0.05881608,0.00035647603,0.0037726425,0.023596011],"study_design_scores_gemma":[0.000027682936,0.00019411334,0.9912914,0.000010625852,0.000043994783,0.0004092818,0.00006552746,0.0011277556,0.0043750545,0.000041815612,0.0023990518,0.00001356242],"about_ca_topic_score_codex":0.00888102,"about_ca_topic_score_gemma":0.023950104,"teacher_disagreement_score":0.00888102,"about_ca_system_score_codex":0.00037475114,"about_ca_system_score_gemma":0.00024605685,"threshold_uncertainty_score":0.01765865},"labels":[],"label_agreement":null},{"id":"W2158891556","doi":"10.1088/0004-637x/757/2/132","title":"FROM THE COLOR-MAGNITUDE DIAGRAM OF ω CENTAURI AND (SUPER-)ASYMPTOTIC GIANT BRANCH STELLAR MODELS TO A GALACTIC PLANE PASSAGE GAS PURGING CHEMICAL EVOLUTION SCENARIO","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Metallicity; Astrophysics; Subgiant; Milky Way; Stars; Nucleosynthesis; Population; Red-giant branch; Stellar evolution; Asymptotic giant branch; Omega; Astronomy; Abundance (ecology); Globular cluster; Biology","score_opus":0.011989623552126266,"score_gpt":0.21184165233428248,"score_spread":0.19985202878215622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158891556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8615743,0.00075334864,0.013672678,0.002171763,0.00023377324,0.000050888313,0.0046442263,0.0028004274,0.11409868],"genre_scores_gemma":[0.9959998,0.00006890947,0.0008885129,0.0000793243,0.000018090648,0.000006982126,0.00077824685,0.00008588608,0.0020742356],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992204,0.000018379375,0.0000025366862,0.000020350362,0.000012066807,0.000024713196],"domain_scores_gemma":[0.9988427,0.00035930445,0.0001129971,0.000082122904,0.00022147023,0.00038134158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036311135,0.0004887892,0.00025245786,0.0011724427,0.00031094352,0.0012639818,0.000588119,0.0008445213,0.02685929],"category_scores_gemma":[0.0012370846,0.0001894329,0.00044162702,0.00039499882,0.00041841538,0.0007033384,0.0005424434,0.00070708146,0.0027004543],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0030067903,0.0005281292,0.23194341,0.00054855435,0.0003617608,0.001814425,0.00218134,0.25734457,0.035074864,0.27788982,0.101350605,0.08795566],"study_design_scores_gemma":[0.0005280272,0.00048044324,0.41130668,0.00022028855,0.00029859666,0.00075397117,0.0021600833,0.41107842,0.004081274,0.1459051,0.023014491,0.00017250639],"about_ca_topic_score_codex":0.00926522,"about_ca_topic_score_gemma":0.0059285536,"teacher_disagreement_score":0.02685929,"about_ca_system_score_codex":0.0004865454,"about_ca_system_score_gemma":0.00021069133,"threshold_uncertainty_score":0.08985323},"labels":[],"label_agreement":null},{"id":"W2158893385","doi":"10.1088/0004-637x/734/2/111","title":"THE COOL ACCRETION DISK IN ESO 243-49 HLX-1: FURTHER EVIDENCE OF AN INTERMEDIATE-MASS BLACK HOLE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Black hole (networking); Accretion (finance); Eddington luminosity; Upper and lower bounds; Accretion disc; Luminosity; Intermediate-mass black hole; Thermal; Supermassive black hole","score_opus":0.026476081578906772,"score_gpt":0.2574786910931902,"score_spread":0.23100260951428345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158893385","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99678516,0.00016192785,0.00031773883,0.00014674626,0.000020758887,0.000020369998,0.00022573535,0.000041723244,0.0022798527],"genre_scores_gemma":[0.99875104,0.00002622028,0.0002446388,0.00013719525,0.000032723412,0.0000073848596,0.00019762504,0.000017342682,0.000585786],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998884,0.0000113728975,0.000006886167,0.00003361218,0.000020099673,0.00003949921],"domain_scores_gemma":[0.99928755,0.00011972936,0.00021302135,0.00006985723,0.000048904018,0.00026090466],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004819255,0.00049328187,0.0011077774,0.00093327824,0.0013721375,0.001373248,0.0010340953,0.0011983778,0.0038629083],"category_scores_gemma":[0.0006092649,0.0003736118,0.00035103748,0.00048094982,0.0009198385,0.00068048533,0.0017668515,0.00096078805,0.00085850665],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.005692925,0.000684463,0.3971866,0.00027251424,0.0003175861,0.032037962,0.00250068,0.0020616816,0.53610355,0.0032036633,0.003162406,0.016776025],"study_design_scores_gemma":[0.00032888594,0.00060739316,0.9825668,0.000028450504,0.00008733246,0.0029817382,0.0007728554,0.003528803,0.0059867054,0.001266907,0.0018115122,0.00003251918],"about_ca_topic_score_codex":0.0016984127,"about_ca_topic_score_gemma":0.0019163123,"teacher_disagreement_score":0.0038629083,"about_ca_system_score_codex":0.00041449585,"about_ca_system_score_gemma":0.00023310297,"threshold_uncertainty_score":0.012922764},"labels":[],"label_agreement":null},{"id":"W2158979907","doi":"10.1088/0004-637x/739/2/99","title":"LOCALIZING COMPACT BINARY INSPIRALS ON THE SKY USING GROUND-BASED GRAVITATIONAL WAVE INTERFEROMETERS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"LIGO; Physics; Gravitational wave; Sky; Observatory; Gravitational-wave observatory; Astronomy; Neutron star; Astrophysics; Astronomical interferometer; Telescope; Interferometry","score_opus":0.08554444302752372,"score_gpt":0.33126570339593353,"score_spread":0.2457212603684098,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2158979907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9818153,0.00006747575,0.017406218,0.00004421721,0.0000021432481,0.000011970632,0.000066385684,0.000045387693,0.00054096524],"genre_scores_gemma":[0.99455607,0.00004359407,0.005196175,0.0000057772286,0.000002770692,0.0000058601427,0.00011338724,0.000003603532,0.0000727938],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99969494,0.00014303425,0.000010728651,0.00007655049,0.000041879935,0.000032892007],"domain_scores_gemma":[0.9971692,0.0014159828,0.0008989485,0.00022203267,0.00016359818,0.00013031682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013520019,0.00021976932,0.00028549152,0.0010892827,0.00030339137,0.0007147023,0.00042303142,0.00031955526,0.00050842634],"category_scores_gemma":[0.006693682,0.00025154772,0.00020934189,0.000864028,0.00046073587,0.0010052056,0.00088127353,0.00023584129,0.0000847378],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051343493,0.0001425518,0.65095407,0.00007969428,0.00021771096,0.00011423965,0.00031409002,0.27577174,0.015516236,0.012034846,0.00046058604,0.043880843],"study_design_scores_gemma":[0.00005635147,0.00014242483,0.1703439,0.000024126715,0.00008817917,0.00008518025,0.00017806824,0.8170048,0.0058977823,0.0056860046,0.00046220387,0.000030961062],"about_ca_topic_score_codex":0.009022445,"about_ca_topic_score_gemma":0.011189084,"teacher_disagreement_score":0.009022445,"about_ca_system_score_codex":0.0006908696,"about_ca_system_score_gemma":0.00047118717,"threshold_uncertainty_score":0.017939866},"labels":[],"label_agreement":null},{"id":"W2159277944","doi":"10.1088/0004-637x/696/1/562","title":"DYNAMICAL AND THERMAL EVOLUTION OF THE QUARK-NOVA EJECTA","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Ejecta; Physics; Breakup; Break-Up; Thermal; Phase (matter); Astrophysics; Nova (rocket); Neutron star; Nuclear physics; Mechanics; Supernova; Thermodynamics","score_opus":0.007393054615536562,"score_gpt":0.2880259688830875,"score_spread":0.28063291426755094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2159277944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99614173,0.00012802413,0.0009814817,0.000037717,0.000004663167,0.0000063546754,0.00011366534,0.000023564417,0.002562794],"genre_scores_gemma":[0.9983436,0.000087275504,0.0005439618,0.000013173401,0.000004032393,0.0000042796296,0.0002515824,0.000023878758,0.00072806654],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994254,0.000008802165,0.0000026041146,0.000014013348,0.00001150284,0.0000206286],"domain_scores_gemma":[0.9998134,0.00003624289,0.000046889985,0.000010863085,0.000019524334,0.00007314462],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020896597,0.00029756528,0.0002720415,0.000450768,0.000488809,0.0007979125,0.0002552672,0.00038685513,0.0012897373],"category_scores_gemma":[0.00078416476,0.0003017408,0.00043462534,0.00031706685,0.00046250125,0.00051127205,0.00093388266,0.00044986463,0.00028741665],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017247205,0.00042000634,0.44724163,0.00014443578,0.0004376554,0.0052523958,0.0014233647,0.26138335,0.24090163,0.019027218,0.0010196026,0.021023983],"study_design_scores_gemma":[0.00012971746,0.00032326896,0.6171157,0.000031215044,0.00008470947,0.0011920788,0.0006277218,0.3583593,0.014355111,0.004962069,0.0027039994,0.00011510164],"about_ca_topic_score_codex":0.0041692564,"about_ca_topic_score_gemma":0.00306785,"teacher_disagreement_score":0.0041692564,"about_ca_system_score_codex":0.0007637434,"about_ca_system_score_gemma":0.00020206913,"threshold_uncertainty_score":0.008289993},"labels":[],"label_agreement":null},{"id":"W2159307499","doi":"10.1088/0004-637x/779/2/163","title":"<i>NuSTAR</i>OBSERVATIONS OF MAGNETAR 1E 1841–045","year":2013,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Magnetar; Astrophysics; Astronomy; Neutron star","score_opus":0.017825953698109125,"score_gpt":0.2173834187864728,"score_spread":0.19955746508836367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2159307499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929149,0.0005265679,0.0011687557,0.00009827376,0.000032846685,0.000010575404,0.0016896388,0.0002396719,0.0033187254],"genre_scores_gemma":[0.9908794,0.00022518018,0.0035602695,0.00010227963,0.000052143805,0.000011654224,0.0042250548,0.000049912378,0.00089423213],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986005,0.000012123593,0.000009155872,0.00003828567,0.00005570772,0.000024625066],"domain_scores_gemma":[0.9995783,0.000022328437,0.00021095984,0.00004752152,0.000055690212,0.00008533251],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003989211,0.00020659929,0.0003123489,0.0010500207,0.00041437,0.00037971183,0.00036593244,0.00026997473,0.00075826346],"category_scores_gemma":[0.00037137838,0.00015841657,0.00031707075,0.0005494368,0.00023259612,0.00016345565,0.00054217485,0.00028643897,0.0004374201],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076927553,0.00021814229,0.734776,0.000456498,0.00051006716,0.0017024985,0.00071112404,0.0032281876,0.20728315,0.0008959738,0.0077937525,0.0416552],"study_design_scores_gemma":[0.000014068461,0.00015782118,0.9824692,0.00002077606,0.000074098716,0.0008887095,0.000063938096,0.0014428666,0.00554982,0.00011519289,0.0091794655,0.000023970888],"about_ca_topic_score_codex":0.0026808504,"about_ca_topic_score_gemma":0.011395469,"teacher_disagreement_score":0.0026808504,"about_ca_system_score_codex":0.00037553848,"about_ca_system_score_gemma":0.00020839075,"threshold_uncertainty_score":0.0053304434},"labels":[],"label_agreement":null},{"id":"W2159338766","doi":"10.1086/533410","title":"Atomic Alignment and Diagnostics of Magnetic Fields in Diffuse Media","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Magnetic field; Hanle effect; Magnetic dipole; Polarization (electrochemistry); Ion; Excited state; Interstellar medium; Dipole; Emission spectrum","score_opus":0.009381184999539875,"score_gpt":0.21299167674466873,"score_spread":0.20361049174512885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2159338766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9684409,0.0011467689,0.021377863,0.00009383442,0.000016509644,0.000019828678,0.0002009193,0.00012794626,0.008575357],"genre_scores_gemma":[0.99409026,0.00036877976,0.004914396,0.000022700142,0.000023772354,0.0000064168553,0.00007368951,0.000009065024,0.0004908309],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99988997,0.000018300954,0.0000028588954,0.000031861895,0.00003477839,0.000022157212],"domain_scores_gemma":[0.9996625,0.00005811576,0.0001647935,0.000026653403,0.00004674736,0.00004121905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014997905,0.00021897742,0.00016121988,0.00089679833,0.00021165215,0.0004083805,0.00024392888,0.00024038854,0.00078139064],"category_scores_gemma":[0.0006320378,0.00014422274,0.000059533133,0.0005558115,0.00039402925,0.000662352,0.0005981666,0.00029415116,0.00018506704],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040013515,0.000045859186,0.07479307,0.00012778243,0.00003964386,0.00041475866,0.00028473735,0.004488256,0.87902117,0.0059020817,0.0003107488,0.034171782],"study_design_scores_gemma":[0.00012261192,0.0006677236,0.3806714,0.00006750853,0.0001018709,0.0023035805,0.0011256521,0.06994462,0.5277741,0.009993849,0.0071209245,0.00010615348],"about_ca_topic_score_codex":0.00049853517,"about_ca_topic_score_gemma":0.0005025611,"teacher_disagreement_score":0.00089679833,"about_ca_system_score_codex":0.00016171318,"about_ca_system_score_gemma":0.00006120949,"threshold_uncertainty_score":0.0026140213},"labels":[],"label_agreement":null},{"id":"W2159346111","doi":"10.1086/428643","title":"On the Anomalous Red Giant Branch of the Globular Cluster ω Centauri","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Horizontal branch; Subgiant; Globular cluster; Physics; Stars; Astrophysics; Red-giant branch; Astronomy; Blue straggler; Red giant; Homogeneous","score_opus":0.00744202952567787,"score_gpt":0.20526930526402962,"score_spread":0.19782727573835174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2159346111","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94632006,0.0036176823,0.00052307046,0.006457546,0.0029625224,0.000012276054,0.0005197334,0.00011279809,0.039474282],"genre_scores_gemma":[0.9907453,0.0008974,0.00015096141,0.0011483713,0.001967113,0.0000043849755,0.0006958684,0.00005093357,0.0043396773],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997929,0.00002321549,0.000008434291,0.00007003902,0.000053131007,0.000052243126],"domain_scores_gemma":[0.99816304,0.00059360353,0.00032853681,0.00025949304,0.0003475374,0.00030776588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005780697,0.00022852891,0.0004070627,0.0014843774,0.001181951,0.0011666513,0.00066088093,0.0010223327,0.004603616],"category_scores_gemma":[0.0029593105,0.00014601773,0.00022475705,0.001325177,0.00083036465,0.0006155047,0.000865512,0.0008482251,0.0015629437],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.010318822,0.0002683877,0.49792457,0.0011632631,0.00055216835,0.012909963,0.002564235,0.0032324702,0.04576699,0.074961856,0.18629171,0.16404554],"study_design_scores_gemma":[0.00019511247,0.0003162669,0.9044132,0.0002819328,0.00028279802,0.0036142985,0.00077283813,0.0028698172,0.004232708,0.025298372,0.057635196,0.000087368026],"about_ca_topic_score_codex":0.0027709855,"about_ca_topic_score_gemma":0.0033150387,"teacher_disagreement_score":0.004603616,"about_ca_system_score_codex":0.00063938973,"about_ca_system_score_gemma":0.00018892206,"threshold_uncertainty_score":0.015400648},"labels":[],"label_agreement":null},{"id":"W2159503116","doi":"10.1086/500666","title":"The Evolution of the Star Formation Activity in Galaxies and Its Dependence on Environment","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":309,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Star formation; Galaxy; Elliptical galaxy; Galaxy group; Redshift; Astronomy; Galaxy cluster; Sky; Stellar mass","score_opus":0.005166305379354278,"score_gpt":0.18488806041357,"score_spread":0.17972175503421572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2159503116","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991554,0.0001028367,0.000075953896,0.00005077016,0.0000010499143,8.8960735e-7,0.0002816026,0.000007333888,0.00032404225],"genre_scores_gemma":[0.9993291,0.0000778051,0.00006402374,0.000009289464,0.000005111128,0.0000010242192,0.00030279226,0.0000034822071,0.0002074405],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999828,0.000047027974,0.00000947396,0.000049302096,0.000024687786,0.00004159587],"domain_scores_gemma":[0.9967631,0.0011500188,0.0011803948,0.0002295831,0.00021383422,0.00046299348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042613962,0.00015161869,0.00017164141,0.00079621153,0.00021046364,0.0008826484,0.00024159969,0.00041401212,0.0016640883],"category_scores_gemma":[0.0023963843,0.0001641737,0.00026653302,0.0010457216,0.00041162458,0.0005452844,0.00039085455,0.0004157442,0.00050187943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006203401,0.000025080022,0.99360067,0.0000070504107,0.000043165695,0.000055872068,0.0001286991,0.0006736856,0.0018143019,0.00014805436,0.00016211183,0.003279157],"study_design_scores_gemma":[9.154579e-7,0.000017568598,0.9989064,0.0000010299948,0.0000063126126,0.000046005523,0.00003627666,0.00072877854,0.00010595179,0.0000389663,0.000110001194,0.0000018005037],"about_ca_topic_score_codex":0.008387418,"about_ca_topic_score_gemma":0.0075532864,"teacher_disagreement_score":0.008387418,"about_ca_system_score_codex":0.00023768762,"about_ca_system_score_gemma":0.00012885025,"threshold_uncertainty_score":0.0166772},"labels":[],"label_agreement":null},{"id":"W2159916197","doi":"10.1088/0004-637x/712/2/1157","title":"FARADAY ROTATION OF THE SUPERNOVA REMNANT G296.5+10.0: EVIDENCE FOR A MAGNETIZED PROGENITOR WIND","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Supernova remnant; Faraday effect; Magnetic field; Rotation (mathematics); Supergiant; Supernova; Interstellar medium; Stellar rotation","score_opus":0.018068755393322544,"score_gpt":0.2596282163136612,"score_spread":0.24155946092033864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2159916197","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985947,0.000054278302,0.0001890083,0.000020070145,0.00000425549,0.0000040592695,0.000109108296,0.000020545936,0.0010039802],"genre_scores_gemma":[0.99913234,0.00002936166,0.0003069881,0.0000138952555,0.000006124642,0.0000022209817,0.00026951442,0.0000067015285,0.00023294344],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995995,0.0000034892005,0.0000027848164,0.000012597993,0.000012230603,0.000008989104],"domain_scores_gemma":[0.9998429,0.00000964853,0.000054945613,0.000015817575,0.00001639923,0.000060199487],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010904374,0.00020136307,0.00019685419,0.00035037912,0.00019161428,0.00032225426,0.00023628672,0.00020531462,0.001296268],"category_scores_gemma":[0.00019386571,0.00017691239,0.00018427396,0.00018778363,0.00022077806,0.00011089242,0.00036174143,0.00019233952,0.00042321088],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071742054,0.00008669409,0.36137438,0.00007929168,0.000101697835,0.00277951,0.0003718418,0.0014907015,0.6239711,0.0004887519,0.00045284812,0.00808575],"study_design_scores_gemma":[0.0000265976,0.00017274731,0.9885886,0.000006620439,0.000022527647,0.0011761287,0.000118436845,0.0017415357,0.0068099727,0.0001665735,0.0011592156,0.000011214097],"about_ca_topic_score_codex":0.0014008612,"about_ca_topic_score_gemma":0.002658938,"teacher_disagreement_score":0.0014008612,"about_ca_system_score_codex":0.00013822786,"about_ca_system_score_gemma":0.000075918586,"threshold_uncertainty_score":0.0043364763},"labels":[],"label_agreement":null},{"id":"W2160004080","doi":"10.1088/0004-637x/767/2/111","title":"CHARACTERIZING THE COOL KOIs. V. KOI-256: A MUTUALLY ECLIPSING POST-COMMON ENVELOPE BINARY","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; White dwarf; Astrophysics; Light curve; Common envelope; Astronomy; Orbital period; Photometry (optics); Occultation; Planet; Circumbinary planet; Transit (satellite); Stars","score_opus":0.010778453307454883,"score_gpt":0.21800198553756098,"score_spread":0.2072235322301061,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2160004080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99763155,0.00007674247,0.00028765242,0.000013239799,0.0000037761072,0.000010098248,0.0004790656,0.000022534548,0.0014752306],"genre_scores_gemma":[0.99598616,0.0000514085,0.0009618979,0.00002473485,0.000007373509,0.000009327338,0.0023988583,0.000018995459,0.00054113904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998809,0.0000037394911,0.00000823713,0.0000538954,0.00002538081,0.000027856233],"domain_scores_gemma":[0.9996536,0.000023457826,0.00014873527,0.000048608388,0.000032090335,0.00009363099],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013446617,0.00023649023,0.00026409404,0.0006678165,0.00040395628,0.0005641962,0.0003202543,0.0002497337,0.0007025208],"category_scores_gemma":[0.00043968152,0.00017401025,0.00014558453,0.0004124746,0.00027346786,0.00030437933,0.0007095849,0.000314963,0.00081541494],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005287098,0.00011095895,0.782347,0.00008393421,0.00004188032,0.0015329175,0.0005432998,0.0003902942,0.19836363,0.000812632,0.0008238872,0.014420843],"study_design_scores_gemma":[0.000017626526,0.00017649058,0.95887035,0.000019160638,0.000049592625,0.004544203,0.00039676955,0.0015382931,0.02677056,0.0003086722,0.00728808,0.000020284177],"about_ca_topic_score_codex":0.0015588751,"about_ca_topic_score_gemma":0.0023876943,"teacher_disagreement_score":0.0015588751,"about_ca_system_score_codex":0.00025927316,"about_ca_system_score_gemma":0.00016255898,"threshold_uncertainty_score":0.00309968},"labels":[],"label_agreement":null},{"id":"W2160110408","doi":"10.1088/0004-637x/757/2/190","title":"ASTEROSEISMOLOGY OF THE OPEN CLUSTERS NGC 6791, NGC 6811, AND NGC 6819 FROM 19 MONTHS OF<i>KEPLER</i>PHOTOMETRY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":161,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science Mission Directorate; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Fonds Wetenschappelijk Onderzoek; Science and Technology Facilities Council; Vlaamse regering; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Asteroseismology; Photometry (optics); Open cluster; Astrophysics; Astronomy; Kepler; Hubble sequence; Stars; Spiral galaxy","score_opus":0.015115127489805709,"score_gpt":0.24494537103908154,"score_spread":0.22983024354927584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2160110408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99621993,0.00019451686,0.000103124425,0.000063742365,0.000010106652,0.0000057836833,0.001626595,0.000016258171,0.001759964],"genre_scores_gemma":[0.99574476,0.0001253711,0.00011327209,0.00001819197,0.000018869501,0.0000054018533,0.0030037528,0.000011215799,0.00095928734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989307,0.000007989449,0.0000074297614,0.000032641477,0.000023491277,0.000035378336],"domain_scores_gemma":[0.9990965,0.000094544375,0.00027856382,0.00007426126,0.0002723897,0.00018373037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002936031,0.00017756067,0.00024151565,0.0017170829,0.0006840511,0.00058979593,0.00019477821,0.0003122182,0.0016236819],"category_scores_gemma":[0.00064910995,0.00011525,0.00024220465,0.0011455707,0.00028692902,0.0005636007,0.0007680799,0.00029855987,0.00038002056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005130586,0.000077362296,0.9696027,0.000036349695,0.000070761555,0.00054109853,0.0009956583,0.0007562608,0.009502137,0.00042296428,0.0022461184,0.015235445],"study_design_scores_gemma":[0.0000025416484,0.000010460835,0.99805874,0.0000041019325,0.000012091864,0.000073463685,0.000116402334,0.00009352548,0.0002955543,0.000038247144,0.0012917944,0.000003161088],"about_ca_topic_score_codex":0.01507876,"about_ca_topic_score_gemma":0.027039468,"teacher_disagreement_score":0.01507876,"about_ca_system_score_codex":0.00054423895,"about_ca_system_score_gemma":0.0002686726,"threshold_uncertainty_score":0.02998197},"labels":[],"label_agreement":null},{"id":"W2160254914","doi":"10.1086/589936","title":"The Relation between Star Formation, Morphology, and Local Density in High‐Redshift Clusters and Groups","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Star formation; Galaxy; Spiral galaxy; Cluster (spacecraft); Redshift; Galaxy cluster; Star cluster; Astronomy; Star (game theory); Stellar mass","score_opus":0.00789755533690225,"score_gpt":0.19652769835474682,"score_spread":0.18863014301784456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2160254914","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99923205,0.00003880376,0.00010158389,0.000012022585,4.220821e-7,0.0000014287232,0.00007813802,0.0000067857163,0.0005286236],"genre_scores_gemma":[0.99969435,0.000014926049,0.00005241528,0.0000025664683,0.0000015005139,0.0000011359683,0.00010277143,0.0000016967155,0.00012857938],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998795,0.000015925687,0.000008097381,0.000035632314,0.000020548998,0.00004037547],"domain_scores_gemma":[0.99805874,0.0004316659,0.0007962355,0.00015287234,0.00019023492,0.00037029435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002171248,0.00015543806,0.00018154425,0.0012486647,0.0003291072,0.0006171383,0.00028193166,0.00024497023,0.0025635178],"category_scores_gemma":[0.0015800581,0.0001585736,0.00019316822,0.0008500419,0.0005000252,0.00041805755,0.00061556604,0.00018184898,0.0003617142],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052808486,0.000008721003,0.9949595,0.000006104142,0.000022753817,0.00003004779,0.00021653937,0.0004765895,0.0025204853,0.00018872404,0.000054214917,0.0014634476],"study_design_scores_gemma":[0.000001351468,0.000012257254,0.9992587,9.536709e-7,0.000004897034,0.00003820416,0.00008280826,0.0003216378,0.00015749174,0.000066881985,0.000053133015,0.0000017004752],"about_ca_topic_score_codex":0.006536719,"about_ca_topic_score_gemma":0.0064840876,"teacher_disagreement_score":0.006536719,"about_ca_system_score_codex":0.000267531,"about_ca_system_score_gemma":0.00008835826,"threshold_uncertainty_score":0.012997329},"labels":[],"label_agreement":null},{"id":"W2160672251","doi":"10.1088/0004-637x/740/1/3","title":"AGN UNIFICATION AT<i>z</i>∼ 1:<i>u</i>–<i>R</i>COLORS AND GRADIENTS IN X-RAY AGN HOSTS","year":2011,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Lawrence Livermore National Laboratory; Space Telescope Science Institute; European Southern Observatory; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Wide Field Camera 3; Active galactic nucleus; Photometry (optics); Extinction (optical mineralogy); Astronomy; Luminosity; Star formation; Hubble space telescope; Stars; Optics","score_opus":0.012465188467032649,"score_gpt":0.2027580156894586,"score_spread":0.19029282722242594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2160672251","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988726,0.000058720227,0.00009062464,0.00002202689,0.0000016209417,0.0000029551527,0.00014272086,0.000021662989,0.00078697543],"genre_scores_gemma":[0.9995672,0.0000150468995,0.00006403918,0.000008491273,0.0000027857786,0.0000016535269,0.0002367003,0.0000048608244,0.00009930168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977916,0.000010133981,0.00000922004,0.000072055,0.000035042263,0.00009447355],"domain_scores_gemma":[0.9989255,0.000100793775,0.0004924046,0.00008755327,0.00009471643,0.000299095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032385642,0.00025725111,0.00032968188,0.0010779636,0.000490605,0.001358656,0.00040742918,0.00031842518,0.002169379],"category_scores_gemma":[0.001112478,0.00025692338,0.00035259486,0.0004838325,0.00039748262,0.00045472148,0.0010983443,0.00041792926,0.00037143007],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001685147,0.00003707009,0.97964555,0.00001289272,0.000037900354,0.00012274494,0.00024416822,0.0010975213,0.012682572,0.00059027487,0.00027209334,0.005088658],"study_design_scores_gemma":[0.0000040284535,0.0000108555405,0.998042,0.00000411716,0.000016702095,0.000052387117,0.000071135124,0.0010180944,0.0005305587,0.000076976314,0.00016997659,0.0000030736132],"about_ca_topic_score_codex":0.013352541,"about_ca_topic_score_gemma":0.01036286,"teacher_disagreement_score":0.013352541,"about_ca_system_score_codex":0.00082903716,"about_ca_system_score_gemma":0.00023080186,"threshold_uncertainty_score":0.026549637},"labels":[],"label_agreement":null},{"id":"W2160696745","doi":"10.1086/522035","title":"Stellar Populations across the NGC 4244 Truncated Galactic Disk","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Stars; Galaxy; Star formation; Astronomy; RADIUS; Angular momentum; Star count; Hubble space telescope; Photometry (optics)","score_opus":0.013846780314832954,"score_gpt":0.25879866438561167,"score_spread":0.24495188407077872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2160696745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943775,0.000028857652,0.00005909979,0.000007393842,8.4532945e-7,0.0000011514618,0.00016201539,0.000013576745,0.0002893014],"genre_scores_gemma":[0.9988883,0.000023786277,0.00024181337,0.000007328285,0.0000021040426,0.0000026065245,0.00063105725,0.0000043769205,0.00019859769],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987304,0.0000118285925,0.0000058580795,0.00004519408,0.000032586115,0.000031582105],"domain_scores_gemma":[0.9996691,0.000024492987,0.00009198506,0.000059249945,0.000049743845,0.00010551662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012998236,0.00027645216,0.00031908034,0.0011073675,0.00041876733,0.00039371313,0.00037661742,0.00031860554,0.0009634289],"category_scores_gemma":[0.0005115767,0.00020860226,0.00021465981,0.00077485066,0.00025688738,0.0002979113,0.0005452852,0.00032842485,0.00025570346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004391644,0.00012037461,0.9161655,0.000031570766,0.00015723887,0.0006953661,0.0007969174,0.005024197,0.06388393,0.000725442,0.00060807867,0.011352185],"study_design_scores_gemma":[0.000010005214,0.000052768322,0.9949255,0.000002397867,0.000015085756,0.00016667694,0.00009632522,0.0030285255,0.000946755,0.00012986796,0.00061944424,0.000006677685],"about_ca_topic_score_codex":0.01774745,"about_ca_topic_score_gemma":0.020444924,"teacher_disagreement_score":0.01774745,"about_ca_system_score_codex":0.00063342025,"about_ca_system_score_gemma":0.00016492132,"threshold_uncertainty_score":0.035288334},"labels":[],"label_agreement":null},{"id":"W2161301892","doi":"10.1088/0004-637x/802/2/105","title":"INFERRING THE STRUCTURE OF THE SOLAR CORONA AND INNER HELIOSPHERE DURING THE MAUNDER MINIMUM USING GLOBAL THERMODYNAMIC MAGNETOHYDRODYNAMIC SIMULATIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Corona (planetary geology); Solar minimum; Heliosphere; Sunspot; Astronomy; Coronal hole; Solar cycle; Solar wind; Magnetic field; Coronal mass ejection","score_opus":0.007927244578255405,"score_gpt":0.2286223780560135,"score_spread":0.22069513347775807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161301892","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966325,0.00003091928,0.0019806805,0.000059455022,0.000003048514,0.0000064243145,0.00019762643,0.000025324036,0.0010639168],"genre_scores_gemma":[0.99907136,0.000017723962,0.0006779829,0.000009191484,0.000003092062,0.0000055932896,0.00012441826,0.0000073566803,0.00008327427],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999529,0.000015224754,0.0000025628049,0.000012883946,0.0000032300854,0.000013269974],"domain_scores_gemma":[0.9998072,0.00008965648,0.000028350889,0.000016479258,0.000014146281,0.000044142525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025666752,0.00030115107,0.00030747446,0.00034802148,0.0003855781,0.00069581345,0.0004705689,0.0006043622,0.0010914432],"category_scores_gemma":[0.0010065449,0.00033049696,0.0005923381,0.00022882762,0.0004096016,0.00046450965,0.000343391,0.00032261023,0.00011007791],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009532996,0.000032812488,0.06496505,0.000018290664,0.00008965283,0.00015788614,0.00007947316,0.9290824,0.0024410486,0.0013869833,0.0001439456,0.0015071838],"study_design_scores_gemma":[0.000042292446,0.000029175399,0.022978555,0.0000062180366,0.000022568407,0.000020037449,0.00006321721,0.97566926,0.00027249413,0.0007400612,0.0001469823,0.000009176053],"about_ca_topic_score_codex":0.020241281,"about_ca_topic_score_gemma":0.0140864495,"teacher_disagreement_score":0.020241281,"about_ca_system_score_codex":0.00071239844,"about_ca_system_score_gemma":0.0005130774,"threshold_uncertainty_score":0.040246964},"labels":[],"label_agreement":null},{"id":"W2161424626","doi":"10.1088/0004-637x/723/1/457","title":"THE DYNAMICS OF DENSE CORES IN THE PERSEUS MOLECULAR CLOUD. II. THE RELATIONSHIP BETWEEN DENSE CORES AND THE CLOUD","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Velocity dispersion; Physics; Dispersion (optics); Kinematics; Molecular cloud; Turbulence; Core (optical fiber); Astrophysics; Scale (ratio); Cloud computing; Line-of-sight; Extinction (optical mineralogy); Length scale; Star formation; Computational physics; Mechanics; Galaxy; Classical mechanics; Optics; Stars","score_opus":0.011654034314501209,"score_gpt":0.2501682600560641,"score_spread":0.23851422574156286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161424626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988757,0.00013389102,0.00014294524,0.000063191794,0.0000012578976,0.0000031625714,0.00020886284,0.000004941829,0.0005660035],"genre_scores_gemma":[0.9994363,0.00006996932,0.0001512863,0.000010981584,0.0000029811963,0.0000017240255,0.0002019837,0.000001705774,0.00012303665],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996483,0.000004701851,0.0000015348786,0.0000107578835,0.000005910697,0.000012208649],"domain_scores_gemma":[0.9997061,0.000058138692,0.00012455384,0.000020591453,0.000032491218,0.000058044177],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001298248,0.00011563076,0.00009201706,0.00045265036,0.0001859167,0.00043549752,0.0002006857,0.00012482073,0.0007069265],"category_scores_gemma":[0.00077314436,0.00010827854,0.000065988934,0.00040071327,0.00029564518,0.00035499735,0.00044107588,0.00014954238,0.000100584526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017634097,0.000042884254,0.95634586,0.000025854757,0.00003872847,0.0003004648,0.00030794414,0.01564219,0.007935859,0.0043327943,0.00071309577,0.014137965],"study_design_scores_gemma":[0.000030155958,0.00003191906,0.9646052,0.000014179512,0.000012891326,0.000111012225,0.0003413989,0.028811874,0.0018012354,0.0027947756,0.0014381869,0.0000071156137],"about_ca_topic_score_codex":0.033059385,"about_ca_topic_score_gemma":0.034120027,"teacher_disagreement_score":0.033059385,"about_ca_system_score_codex":0.00076660205,"about_ca_system_score_gemma":0.00027315933,"threshold_uncertainty_score":0.06573391},"labels":[],"label_agreement":null},{"id":"W2161947325","doi":"10.1086/339318","title":"Magnetic Fields in Star‐forming Molecular Clouds. III. Submillimeter Polarimetry of Intermediate‐Mass Cores and Filaments in Orion B","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McMaster University","funders":"","keywords":"Polarization (electrochemistry); Magnetic field; Polarimeter; Polarimetry; Submillimeter Array; Perpendicular; Linear polarization; Protein filament; Bent molecular geometry; Ionization","score_opus":0.008220123937973885,"score_gpt":0.21939815425143527,"score_spread":0.21117803031346138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161947325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995788,0.00003702651,0.000085229265,0.0000071384998,6.1783606e-7,0.0000010436414,0.000028974107,0.000003947864,0.00025727073],"genre_scores_gemma":[0.99961483,0.000030282237,0.00018581636,0.000004288092,0.0000024651692,0.0000016638658,0.000087105494,0.0000013042605,0.00007219357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996793,0.000003832738,0.0000013934257,0.00000725371,0.000007576304,0.000011867682],"domain_scores_gemma":[0.99982315,0.000017499868,0.0000846728,0.000009938835,0.000026373862,0.000038510676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000066440596,0.00012113104,0.000076249504,0.00037530958,0.00024708066,0.00030906324,0.000167869,0.00015055377,0.00032413288],"category_scores_gemma":[0.0003005785,0.00011217301,0.00007837808,0.00022924121,0.00017181237,0.0001517674,0.00021361181,0.00013158673,0.000093544535],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002671151,0.000047744714,0.7865584,0.000033005632,0.000034536504,0.0002761844,0.00046773322,0.0018620861,0.20093764,0.00040012685,0.000120413955,0.008995101],"study_design_scores_gemma":[0.000016495973,0.00005336058,0.9888954,0.000007536428,0.000013602685,0.00012497242,0.0001537646,0.0025021029,0.0075191087,0.00013747452,0.0005717806,0.000004468291],"about_ca_topic_score_codex":0.0062646195,"about_ca_topic_score_gemma":0.0055164737,"teacher_disagreement_score":0.0062646195,"about_ca_system_score_codex":0.0003297947,"about_ca_system_score_gemma":0.00010045274,"threshold_uncertainty_score":0.012456298},"labels":[],"label_agreement":null},{"id":"W2161960153","doi":"10.1086/422165","title":"Magnetic Effects at the Edge of the Solar System: MHD Instabilities, the de Laval Nozzle Effect, and an Extended Jet","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Magnetohydrodynamics; Magnetohydrodynamic drive; Heliosphere; Jet (fluid); Heliospheric current sheet; Magnetic field; Interplanetary magnetic field; Solar wind; Turbulence; Solar rotation","score_opus":0.002889159116431309,"score_gpt":0.2026050886379988,"score_spread":0.1997159295215675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2161960153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9861573,0.00054638245,0.005517138,0.00035369725,0.00006395468,0.000019144529,0.00019132713,0.00015172838,0.006999329],"genre_scores_gemma":[0.9979438,0.00009961788,0.0013543948,0.000051852287,0.0000219363,0.000006139981,0.00005189968,0.00001974637,0.000450604],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999186,0.000023917592,0.000005525906,0.000011030567,0.00001949788,0.000021422074],"domain_scores_gemma":[0.99982446,0.00004958943,0.000037503207,0.000020770063,0.000020465553,0.000047179103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019176856,0.00037249242,0.00041399317,0.00022363995,0.00043997375,0.0008123577,0.0007653331,0.0007985161,0.0012614784],"category_scores_gemma":[0.0006599413,0.0002041675,0.0005354538,0.00021214676,0.00044713853,0.00061454513,0.0006311072,0.0004952911,0.000111166635],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031578186,0.00015327647,0.026591232,0.00010355678,0.00016195013,0.0018635619,0.00022252052,0.9305649,0.029169844,0.005439009,0.0007226785,0.0046917545],"study_design_scores_gemma":[0.00017589919,0.00008425637,0.016499603,0.000017886992,0.000032786364,0.00018698371,0.0000643057,0.97797865,0.0028018004,0.0011912615,0.0009420198,0.000024580877],"about_ca_topic_score_codex":0.009604366,"about_ca_topic_score_gemma":0.0034433785,"teacher_disagreement_score":0.009604366,"about_ca_system_score_codex":0.000523891,"about_ca_system_score_gemma":0.00031331522,"threshold_uncertainty_score":0.019096911},"labels":[],"label_agreement":null},{"id":"W2162106564","doi":"10.1088/0004-637x/691/1/l13","title":"THE JUNE 2008 FLARE OF MARKARIAN 421 FROM OPTICAL TO TeV ENERGIES","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Instituto de Astrofísica de Canarias; Georgian National Science Foundation; Max-Planck-Gesellschaft; Bundesministerium für Bildung und Forschung; U.S. Department of Energy; Helmholtz-Gemeinschaft; National Science Foundation; Science Foundation Ireland; Smithsonian Institution","keywords":"Physics; Astrophysics; Blazar; Flare; Egret; Flux (metallurgy); Spectral energy distribution; Photon; Synchrotron; MAGIC (telescope); Gamma ray; Astronomy; Galaxy; Nuclear physics; Optics","score_opus":0.007391120331629513,"score_gpt":0.2029068735192749,"score_spread":0.19551575318764539,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162106564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963206,0.00009985434,0.00008636531,0.000082235994,0.00001040389,0.0000037558839,0.00030384416,0.00003406473,0.0030588447],"genre_scores_gemma":[0.9977864,0.000045818546,0.00017889704,0.00007087641,0.000021915885,0.0000017129754,0.00072120887,0.000008371836,0.0011647944],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991643,0.000003365294,0.0000022731058,0.000020687501,0.000028397582,0.000028814013],"domain_scores_gemma":[0.9998963,0.000005123563,0.00003879113,0.000009371693,0.000016937138,0.000033583223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007927528,0.00014429205,0.00019400143,0.00033686255,0.000382209,0.00049266795,0.00013837172,0.00025327876,0.0010807146],"category_scores_gemma":[0.0001403829,0.000097972545,0.000116178504,0.00022024257,0.00013969041,0.00017028741,0.00044546035,0.00032336835,0.00037430768],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016041594,0.00028795173,0.71603495,0.00016271399,0.00021402963,0.00839518,0.0023879928,0.0015638004,0.19846909,0.00095798005,0.009177141,0.060744967],"study_design_scores_gemma":[0.000006209648,0.00008050966,0.9886497,0.0000067836577,0.000012183552,0.00066572294,0.00016962994,0.00022853237,0.003253395,0.000043862103,0.0068748733,0.000008517519],"about_ca_topic_score_codex":0.004335726,"about_ca_topic_score_gemma":0.012525248,"teacher_disagreement_score":0.004335726,"about_ca_system_score_codex":0.000346565,"about_ca_system_score_gemma":0.000116382536,"threshold_uncertainty_score":0.008620977},"labels":[],"label_agreement":null},{"id":"W2162210754","doi":"10.1088/0004-637x/776/1/4","title":"THE GEMINI NICI PLANET-FINDING CAMPAIGN: THE FREQUENCY OF GIANT PLANETS AROUND YOUNG B AND A STARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":157,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Planet; Brown dwarf; Stars; Astrometry; Exoplanet; Astronomy; Astrophysics; Giant planet; Planetary system; Planetary mass; Gas giant","score_opus":0.011419319059660529,"score_gpt":0.2177170280296831,"score_spread":0.20629770897002256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162210754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.61245865,0.0068527604,0.0017081082,0.0033054724,0.0005825954,0.00029293678,0.33683094,0.0011211945,0.036847293],"genre_scores_gemma":[0.572511,0.003411584,0.004546096,0.0008785204,0.0008778819,0.00024961823,0.40436408,0.00044159242,0.012719556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960595,0.000054544103,0.00003328105,0.000093511415,0.00015861746,0.000054141416],"domain_scores_gemma":[0.99812144,0.00017560208,0.0005377222,0.00024061708,0.0004202067,0.00050436275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001069703,0.0002962281,0.00029938619,0.0032624586,0.0006808862,0.0007224869,0.00047884535,0.0004074523,0.0022932398],"category_scores_gemma":[0.0018328453,0.0001764836,0.00023329306,0.0030195538,0.00019342366,0.0006301026,0.0013680747,0.00036703242,0.0020144235],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078059937,0.0001067736,0.6145256,0.0006305873,0.00017993379,0.00027929794,0.00094225624,0.00028213995,0.010445116,0.000582707,0.27590376,0.09534123],"study_design_scores_gemma":[0.000029020357,0.00003584643,0.9610907,0.00003450551,0.00003250674,0.00011452767,0.00014564817,0.00023554095,0.0007837036,0.000056073543,0.037429508,0.000012498211],"about_ca_topic_score_codex":0.03890959,"about_ca_topic_score_gemma":0.059584696,"teacher_disagreement_score":0.03890959,"about_ca_system_score_codex":0.0006945735,"about_ca_system_score_gemma":0.0006652149,"threshold_uncertainty_score":0.07736623},"labels":[],"label_agreement":null},{"id":"W2162253853","doi":"10.1088/0004-637x/704/1/564","title":"THE ROADMAP FOR UNIFICATION IN GALAXY GROUP SELECTION. I. A SEARCH FOR EXTENDED X-RAY EMISSION IN THE CNOC2 SURVEY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; McMaster University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Redshift; Luminosity; Galaxy group; Cosmology; Galaxy formation and evolution; Extragalactic astronomy; Velocity dispersion","score_opus":0.01693640868026665,"score_gpt":0.265100838036355,"score_spread":0.24816442935608835,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162253853","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.15629397,0.19616082,0.29332718,0.27370656,0.006417863,0.0026382718,0.015068536,0.008296781,0.04809006],"genre_scores_gemma":[0.33804926,0.035261158,0.5553186,0.02927346,0.0062307687,0.0031588543,0.022058615,0.0012811081,0.009368234],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.98870695,0.004292277,0.0008157531,0.0024498058,0.0017981166,0.0019371393],"domain_scores_gemma":[0.90387726,0.032814216,0.0066530867,0.02367889,0.018,0.014976608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.059976947,0.001491613,0.0028630814,0.00832125,0.0019671277,0.0055218576,0.0070373123,0.0049334094,0.012934011],"category_scores_gemma":[0.037715007,0.0009051835,0.0022511284,0.0043874094,0.0035586215,0.011102164,0.01150251,0.0046283472,0.0052807103],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008556311,0.000399303,0.12820461,0.0016721517,0.00028479096,0.00014093643,0.0010111614,0.0020076078,0.005337293,0.04408042,0.056501377,0.7595046],"study_design_scores_gemma":[0.00040385142,0.0012147829,0.2594965,0.0033134425,0.00031515528,0.000596654,0.0032131267,0.019591833,0.0026396327,0.21606007,0.49278402,0.00037097008],"about_ca_topic_score_codex":0.017538307,"about_ca_topic_score_gemma":0.010320402,"teacher_disagreement_score":0.059976947,"about_ca_system_score_codex":0.0037776865,"about_ca_system_score_gemma":0.008225974,"threshold_uncertainty_score":0.3171922},"labels":[],"label_agreement":null},{"id":"W2162331089","doi":"10.1088/0004-637x/716/1/315","title":"SEARCHING FOR TROJAN ASTEROIDS IN THE HD 209458 SYSTEM: SPACE-BASED<i>MOST</i>PHOTOMETRY AND DYNAMICAL MODELING","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Trojan; Asteroid; Orbit (dynamics); Transit (satellite); Solar System; Stars; Planet","score_opus":0.012235390635174941,"score_gpt":0.24451511038604828,"score_spread":0.23227971975087333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162331089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99872786,0.000023211314,0.000920372,0.0000195986,0.0000010993853,0.0000025333886,0.000062871695,0.000014520117,0.00022784554],"genre_scores_gemma":[0.99900764,0.000015837162,0.0007370818,0.000005861992,0.0000019428048,0.0000020795362,0.00015547717,0.000005118638,0.00006897652],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993813,0.000015447626,0.0000040982436,0.000020932071,0.000008933768,0.000012487648],"domain_scores_gemma":[0.99978,0.0000661249,0.000064091444,0.000026675429,0.000024654251,0.000038425187],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031869183,0.00020503778,0.00018561435,0.00041483383,0.00031888697,0.00040073157,0.00036407064,0.0002078373,0.00036192458],"category_scores_gemma":[0.00067221606,0.0001878361,0.00032489738,0.0002773717,0.00015557921,0.0003068741,0.00023755667,0.00018020146,0.000093425704],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013244097,0.000095426774,0.85627764,0.00003183015,0.00013732979,0.0002133246,0.00019363742,0.12281262,0.012570498,0.001062062,0.00021772672,0.0062553883],"study_design_scores_gemma":[0.000023040993,0.00007289428,0.34719503,0.000009169217,0.000048218102,0.00016098212,0.00011797308,0.6476642,0.0035395017,0.00051666895,0.00063342735,0.00001896009],"about_ca_topic_score_codex":0.012912296,"about_ca_topic_score_gemma":0.0122795375,"teacher_disagreement_score":0.012912296,"about_ca_system_score_codex":0.00051158207,"about_ca_system_score_gemma":0.00027198964,"threshold_uncertainty_score":0.025674284},"labels":[],"label_agreement":null},{"id":"W2162338384","doi":"10.1088/0004-637x/794/2/143","title":"SpeX SPECTROSCOPY OF UNRESOLVED VERY LOW MASS BINARIES. II. IDENTIFICATION OF 14 CANDIDATE BINARIES WITH LATE-M/EARLY-L AND T DWARF COMPONENTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Stellar classification; Brown dwarf; Low Mass; Binary number; Spectral line; Stars; Spectroscopy; Binary star; Radial velocity","score_opus":0.006325321242310631,"score_gpt":0.20428907776707644,"score_spread":0.1979637565247658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162338384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936591,0.00024490827,0.0021826334,0.000029662782,0.000005065768,0.000022188724,0.0012267359,0.00013546832,0.002494311],"genre_scores_gemma":[0.990369,0.00015853648,0.0053945445,0.000040597934,0.000008320813,0.000019045588,0.003067882,0.000026592143,0.0009155781],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998215,0.000015599393,0.000013390823,0.00006385079,0.00006282168,0.000022900205],"domain_scores_gemma":[0.9996537,0.000051859904,0.00011683177,0.000060440037,0.000060233746,0.000057069185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046750339,0.00025554505,0.0001982598,0.0015537492,0.00041670795,0.00033569703,0.00040149537,0.00030825372,0.0017757196],"category_scores_gemma":[0.000459399,0.00017687748,0.00021983052,0.0011455286,0.00017764854,0.00045088,0.0006295495,0.0002148779,0.00055897894],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010304139,0.00031334648,0.5006368,0.00027810168,0.00016324481,0.0005092556,0.00041442915,0.0024814736,0.4188287,0.001014929,0.0018989753,0.07243033],"study_design_scores_gemma":[0.000028961807,0.00022519937,0.9635992,0.000015187735,0.0000598359,0.00067637017,0.0001469002,0.0052143317,0.027870262,0.00036922286,0.0017814178,0.000013173807],"about_ca_topic_score_codex":0.00089114497,"about_ca_topic_score_gemma":0.0016102216,"teacher_disagreement_score":0.0017757196,"about_ca_system_score_codex":0.0002236248,"about_ca_system_score_gemma":0.00013533367,"threshold_uncertainty_score":0.005940318},"labels":[],"label_agreement":null},{"id":"W2162360520","doi":"10.1088/0004-637x/809/2/165","title":"<i>XMM-NEWTON</i>OBSERVATIONS OF SGR 1806–20 OVER SEVEN YEARS FOLLOWING THE 2004 GIANT FLARE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Flare; Magnetar; Spectral line; Decoupling (probability); Spectral analysis; Accretion (finance); Field line; Giant star","score_opus":0.027294014160983014,"score_gpt":0.31617203424854834,"score_spread":0.2888780200875653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162360520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965125,0.00035145102,0.00019264486,0.0000614875,0.000014357503,0.000012482714,0.001410935,0.00004749723,0.0013966531],"genre_scores_gemma":[0.9917368,0.00024638895,0.000884842,0.000089113964,0.00006156053,0.000021055468,0.0058615813,0.000019109033,0.0010793464],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983096,0.000012694147,0.000018520586,0.000044622582,0.00005590599,0.000037348545],"domain_scores_gemma":[0.99915826,0.000044418204,0.000506919,0.000046786296,0.00012430253,0.00011929833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002963103,0.00028862298,0.0003336905,0.0019165175,0.0004887345,0.00048430724,0.0003313816,0.0005607145,0.0005206036],"category_scores_gemma":[0.0004826806,0.00011897321,0.00029422462,0.0010200118,0.00025040534,0.00028590419,0.00058227836,0.00028896602,0.00039820664],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025073666,0.00013258206,0.9659868,0.00007871141,0.00014158706,0.0009804915,0.000627689,0.00042651824,0.015401094,0.000092061666,0.0021091828,0.0137725705],"study_design_scores_gemma":[0.0000014681543,0.000043667667,0.99752337,0.0000040526957,0.000009754081,0.0002096646,0.000060239727,0.00008434505,0.00044484308,0.000009065724,0.0016045797,0.0000049080845],"about_ca_topic_score_codex":0.0067397337,"about_ca_topic_score_gemma":0.022159806,"teacher_disagreement_score":0.0067397337,"about_ca_system_score_codex":0.00040361253,"about_ca_system_score_gemma":0.00016584227,"threshold_uncertainty_score":0.0134010315},"labels":[],"label_agreement":null},{"id":"W2162431009","doi":"10.1088/0004-637x/738/1/38","title":"CONSTRAINING THE STRUCTURE OF SAGITTARIUS A*'s ACCRETION FLOW WITH MILLIMETER VERY LONG BASELINE INTERFEROMETRY CLOSURE PHASES","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Very-long-baseline interferometry; Physics; Supermassive black hole; Astrophysics; Accretion (finance); Millimeter; Amplitude; Astronomy; Optics; Galaxy","score_opus":0.018574112088488217,"score_gpt":0.22350394097412749,"score_spread":0.20492982888563926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162431009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97264004,0.00031374538,0.021725824,0.0002366421,0.000023685197,0.000031366028,0.00022917532,0.0002285367,0.004571059],"genre_scores_gemma":[0.996573,0.00006617418,0.0029418056,0.000020555304,0.000012254073,0.000010834147,0.0002547414,0.000024953815,0.000095769756],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998266,0.000045112018,0.000012433616,0.000053149117,0.00003198805,0.000030842308],"domain_scores_gemma":[0.9993001,0.00016317566,0.00027438102,0.000111795634,0.000046637455,0.00010393731],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007074617,0.00042767893,0.0002886246,0.00048938853,0.0005198791,0.0012978857,0.0006151335,0.00046965314,0.0006042079],"category_scores_gemma":[0.0026447377,0.00031968692,0.00044074006,0.00042564655,0.0004587159,0.0007811338,0.00078110624,0.000515264,0.00018346416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007230287,0.0002009137,0.64178115,0.00012329125,0.00022254862,0.00044985776,0.00072566996,0.18317777,0.07919807,0.03238489,0.0024170734,0.05859577],"study_design_scores_gemma":[0.00011245189,0.00019248795,0.29661322,0.00006122317,0.000056489596,0.00021883207,0.0002632712,0.6728349,0.007852867,0.015100478,0.0065999655,0.00009382222],"about_ca_topic_score_codex":0.013083413,"about_ca_topic_score_gemma":0.00815429,"teacher_disagreement_score":0.013083413,"about_ca_system_score_codex":0.0011857959,"about_ca_system_score_gemma":0.00069734926,"threshold_uncertainty_score":0.026014507},"labels":[],"label_agreement":null},{"id":"W2162504102","doi":"10.1086/312787","title":"[ITAL]Far Ultraviolet Spectroscopic Explorer[/ITAL] Observations of the Stellar Winds of Two O7 Supergiants in the Magellanic Clouds","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Supergiant; Physics; Astrophysics; Stellar atmosphere; Spectral line; Line (geometry); Hydrostatic equilibrium; Ultraviolet; Astronomy; O-type star; Stars; Optics","score_opus":0.019062663695711943,"score_gpt":0.2383714904747958,"score_spread":0.21930882677908387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162504102","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9744393,0.00013989178,0.00032439915,0.00016948732,0.00003250983,0.000018119483,0.009537319,0.0001469326,0.01519205],"genre_scores_gemma":[0.95191187,0.00032591145,0.0028938085,0.00035012944,0.00008669148,0.000039261115,0.030020136,0.00006805393,0.01430417],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999788,0.0000015626408,0.00000105333,0.0000049683076,0.0000065515273,0.0000070590595],"domain_scores_gemma":[0.9998933,0.000013527772,0.000036756202,0.000008842976,0.000014639736,0.00003291432],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000054187836,0.00013366068,0.00009200749,0.0005880477,0.00026208986,0.00016426954,0.00013296673,0.000165059,0.011971888],"category_scores_gemma":[0.000092312,0.000055121018,0.000085989086,0.0003670466,0.00008594326,0.00012773884,0.00026607446,0.00013608148,0.0020107084],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005755513,0.0002795962,0.7698002,0.00018265766,0.00015584326,0.0022448227,0.00063398434,0.0005334047,0.07511751,0.00096304197,0.05943014,0.09008324],"study_design_scores_gemma":[0.000019535617,0.000087187196,0.98070234,0.00001691123,0.00001628659,0.0006599607,0.00021894228,0.0002551367,0.0016200849,0.000121411504,0.016277518,0.00000463248],"about_ca_topic_score_codex":0.0036135332,"about_ca_topic_score_gemma":0.011995589,"teacher_disagreement_score":0.011971888,"about_ca_system_score_codex":0.000063488704,"about_ca_system_score_gemma":0.000053903186,"threshold_uncertainty_score":0.04004997},"labels":[],"label_agreement":null},{"id":"W2162508614","doi":"10.1088/0004-637x/699/2/1541","title":"UNUSUAL DUST EMISSION FROM PLANETARY NEBULAE IN THE MAGELLANIC CLOUDS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Planetary nebula; Emission spectrum; Spectral line; Large Magellanic Cloud; Spitzer Space Telescope; Infrared; Cosmic dust; Thermal emission; Hubble space telescope","score_opus":0.01019320188957694,"score_gpt":0.23395549517530617,"score_spread":0.22376229328572922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162508614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995559,0.00013062176,0.00008195863,0.0000040943455,7.577238e-7,0.0000021900055,0.00006072796,0.0000052867817,0.000158577],"genre_scores_gemma":[0.9992422,0.00008352133,0.00021076908,0.000008122164,0.000008769666,0.0000028210502,0.00033598594,0.0000020864895,0.00010567454],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988127,0.00000668773,0.0000060234443,0.000042306387,0.000029892113,0.00003367425],"domain_scores_gemma":[0.99985325,0.000016985565,0.000045553767,0.000012585819,0.000015848724,0.000055763147],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106467436,0.00027685516,0.00021259607,0.001502189,0.00040649442,0.00036831494,0.00033947552,0.00021400687,0.0005456536],"category_scores_gemma":[0.00022509503,0.00013104279,0.00019423038,0.00081166445,0.00022834766,0.00017435687,0.00034112117,0.00009341786,0.000119537224],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008237931,0.000060885253,0.94777524,0.000030670195,0.00006631229,0.0008777344,0.00036129836,0.00018288505,0.040889498,0.000054228327,0.00012221393,0.009496656],"study_design_scores_gemma":[0.0000027860253,0.000038094568,0.99690825,0.0000021008575,0.000011473854,0.00073334586,0.00006681929,0.0001862139,0.0015817937,0.000023946106,0.00044354564,0.0000016801458],"about_ca_topic_score_codex":0.0024698596,"about_ca_topic_score_gemma":0.0036979846,"teacher_disagreement_score":0.0024698596,"about_ca_system_score_codex":0.00022079068,"about_ca_system_score_gemma":0.00007692792,"threshold_uncertainty_score":0.004910946},"labels":[],"label_agreement":null},{"id":"W2162596494","doi":"10.1088/0004-637x/807/2/128","title":"THE SCUBA-2 COSMOLOGY LEGACY SURVEY: ALMA RESOLVES THE BRIGHT-END OF THE SUB-MILLIMETER NUMBER COUNTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"FP7 Space; National Institutes of Natural Sciences; Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Foundation; Vetenskapsrådet; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Council; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Millimeter; Galaxy; Flux (metallurgy); Luminous infrared galaxy; Astronomy; Star formation; Cosmology; James Clerk Maxwell Telescope; Luminosity","score_opus":0.016206173263367697,"score_gpt":0.23585343292626074,"score_spread":0.21964725966289303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162596494","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.921951,0.0006682947,0.00747389,0.00019454626,0.000042471478,0.00008940252,0.041864567,0.0017303411,0.025985532],"genre_scores_gemma":[0.9521505,0.00023349083,0.010120883,0.00017541558,0.00010073663,0.00011097538,0.03311182,0.00021781867,0.003778323],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997563,0.000031084564,0.000012531232,0.00006189614,0.000086863874,0.000051388924],"domain_scores_gemma":[0.99869484,0.00014704421,0.00044757876,0.00027718933,0.00022203122,0.00021142286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002220682,0.00031371452,0.00028857836,0.002909553,0.0002793028,0.00065337046,0.00045980836,0.0001908743,0.005460533],"category_scores_gemma":[0.0009457614,0.00017770192,0.00029744927,0.0023058262,0.00017491904,0.00035652154,0.00066890026,0.00028477004,0.0023953426],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032517142,0.000103421786,0.8727414,0.00018749318,0.00017001391,0.00033772195,0.00072540337,0.0021620987,0.022144884,0.0021914626,0.0319985,0.06691241],"study_design_scores_gemma":[0.000012363503,0.000018363979,0.981645,0.000012536062,0.000013920745,0.00012968144,0.00006466162,0.0017885121,0.001240884,0.00033247814,0.014730023,0.000011472317],"about_ca_topic_score_codex":0.011286334,"about_ca_topic_score_gemma":0.024005102,"teacher_disagreement_score":0.011286334,"about_ca_system_score_codex":0.00028984703,"about_ca_system_score_gemma":0.000197682,"threshold_uncertainty_score":0.022441328},"labels":[],"label_agreement":null},{"id":"W2162844870","doi":"10.1088/0004-637x/694/2/l120","title":"WHAT ARE S0 GALAXIES?","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Elliptical galaxy; Peculiar galaxy; Lenticular galaxy; Spiral galaxy; Galaxy; Luminous infrared galaxy; Disc; Galaxy group","score_opus":0.007762717156655229,"score_gpt":0.21613411161765542,"score_spread":0.2083713944610002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2162844870","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9413762,0.010547834,0.00083854015,0.012288407,0.0002442016,0.000021622078,0.0005989831,0.00007399946,0.03401024],"genre_scores_gemma":[0.99151903,0.00298226,0.00036636012,0.0017496758,0.00031713233,0.000008228713,0.00035533638,0.000009811787,0.0026920538],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996061,0.00009268183,0.000020475001,0.00008861812,0.000081753766,0.00011045819],"domain_scores_gemma":[0.99768,0.0005119859,0.0006269978,0.00012953955,0.0003222362,0.0007293445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010327406,0.00020734702,0.00026870205,0.001571995,0.0007578456,0.001998267,0.00047677782,0.0010859646,0.0064031323],"category_scores_gemma":[0.0036393483,0.00016007014,0.0002217339,0.0011629089,0.0020032371,0.0027731129,0.00043950195,0.0004473498,0.0022069141],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023158274,0.0001313327,0.76595175,0.0003303524,0.00007213388,0.0006136481,0.005282597,0.00011391224,0.0018666852,0.022668857,0.013180725,0.18955642],"study_design_scores_gemma":[0.000023732904,0.00020745912,0.90573955,0.00025142732,0.000045129622,0.0030929572,0.010242877,0.00026190822,0.00069670955,0.02982279,0.049586486,0.000028930292],"about_ca_topic_score_codex":0.0057082833,"about_ca_topic_score_gemma":0.0032080226,"teacher_disagreement_score":0.0064031323,"about_ca_system_score_codex":0.00075696065,"about_ca_system_score_gemma":0.00042584035,"threshold_uncertainty_score":0.021420538},"labels":[],"label_agreement":null},{"id":"W2163068820","doi":"10.1088/0004-637x/777/2/103","title":"SHATTERING FLARES DURING CLOSE ENCOUNTERS OF NEUTRON STARS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Neutron star; Astrophysics; Stars; Gravitational wave; Astronomy","score_opus":0.007401200189625593,"score_gpt":0.27611797613802724,"score_spread":0.26871677594840165,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163068820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972812,0.00022670005,0.00081914064,0.0000156293,0.00000769377,0.0000060038637,0.00008333334,0.000027038303,0.0015332894],"genre_scores_gemma":[0.9994419,0.00004294165,0.0002491764,0.0000075652665,0.000007270313,0.0000018534815,0.00011662303,0.000003923121,0.00012879136],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983656,0.000016143065,0.0000072066996,0.000043136,0.00005341591,0.000043609856],"domain_scores_gemma":[0.9992793,0.00016260355,0.00031748423,0.000068222165,0.000057986486,0.00011440392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024027558,0.00015334028,0.00023436877,0.0005667801,0.00049193355,0.00030316814,0.00023795996,0.00037951514,0.0009384732],"category_scores_gemma":[0.0014866246,0.00008012383,0.00014015952,0.00034034075,0.00020255407,0.00036910776,0.00074982183,0.0003273945,0.00023410011],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011394001,0.00013831155,0.777204,0.00019959225,0.00023253195,0.0051055825,0.0022227059,0.0057861996,0.130679,0.0012930834,0.0015368103,0.0744629],"study_design_scores_gemma":[0.000015163687,0.0003399574,0.9735877,0.000026363245,0.00005077124,0.003890992,0.00050805876,0.009669198,0.008220879,0.000781634,0.002877096,0.00003201195],"about_ca_topic_score_codex":0.0010121622,"about_ca_topic_score_gemma":0.0018584959,"teacher_disagreement_score":0.0010121622,"about_ca_system_score_codex":0.00018966514,"about_ca_system_score_gemma":0.00006658045,"threshold_uncertainty_score":0.0031394958},"labels":[],"label_agreement":null},{"id":"W2163098163","doi":"10.1086/505557","title":"A Measurement of the Polarization‐Temperature Angular Cross‐Power Spectrum of the Cosmic Microwave Background from the 2003 Flight of BOOMERANG","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":153,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Leverhulme Trust; National Energy Research Scientific Computing Center; Jet Propulsion Laboratory; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Cosmic microwave background; Bolometer; Physics; Polarization (electrochemistry); Spectral line; Spectral density; Microwave; COSMIC cancer database; Detector; Optics; Astrophysics; Astronomy; Statistics; Chemistry","score_opus":0.005231488188169939,"score_gpt":0.2100786081641716,"score_spread":0.20484711997600166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163098163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968966,0.00007006,0.00061526406,0.000029743625,0.0000065039726,0.000008735775,0.0009665016,0.000057648638,0.0013489636],"genre_scores_gemma":[0.9973484,0.000052441705,0.0006413424,0.000017802093,0.000011903495,0.000008072963,0.0016857802,0.000018332035,0.00021586115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998492,0.000016186897,0.0000037499897,0.000047317793,0.000043986496,0.000039575785],"domain_scores_gemma":[0.9996306,0.00003131478,0.00013288051,0.0000444445,0.000071249575,0.00008948161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017885803,0.00042721952,0.00021852735,0.0010820393,0.00040051676,0.0003999456,0.00024561104,0.0002559676,0.00061531854],"category_scores_gemma":[0.00041266158,0.00019405007,0.00017225656,0.0009486376,0.0002508986,0.00015999537,0.0003373401,0.00044221725,0.000242249],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009308636,0.00022501222,0.8469612,0.000076107404,0.00028114324,0.0005946506,0.00078054774,0.0019928382,0.120838985,0.0003847723,0.0016814438,0.025252312],"study_design_scores_gemma":[0.000008200714,0.00006160909,0.9940546,0.0000032458602,0.000022795213,0.00018198011,0.000027291511,0.0007421595,0.0041375766,0.000035944147,0.0007139593,0.000010662323],"about_ca_topic_score_codex":0.011596848,"about_ca_topic_score_gemma":0.026541691,"teacher_disagreement_score":0.011596848,"about_ca_system_score_codex":0.00048024798,"about_ca_system_score_gemma":0.00016782132,"threshold_uncertainty_score":0.023058712},"labels":[],"label_agreement":null},{"id":"W2163401833","doi":"10.1086/429316","title":"Fourier Transform Emission Spectra of the (000)–(000) Band of the λ4051.6 Band of C<sub>3</sub>","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atomic and Molecular Physics","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Excited state; Spectral line; Emission spectrum; Fourier transform; Helium; Microwave; Spectrometer; Atomic physics; Fourier transform spectroscopy; Torr; Analytical Chemistry (journal); Optics; Astronomy","score_opus":0.004510771099605051,"score_gpt":0.20249510800156012,"score_spread":0.19798433690195508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163401833","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9817925,0.00024927515,0.007874915,0.00011996967,0.000013564642,0.000012252518,0.00096637796,0.00023620577,0.008734837],"genre_scores_gemma":[0.9839702,0.00023495087,0.008654532,0.00005525976,0.000008684453,0.000015194189,0.0010222106,0.00006754309,0.005971482],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999374,0.000003777277,0.0000012247036,0.000012130521,0.000034964414,0.000010593605],"domain_scores_gemma":[0.9998622,0.000038549548,0.000022504932,0.0000127287285,0.000040719035,0.000023251376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011877744,0.000148802,0.00010853977,0.00034210098,0.000285699,0.000120078636,0.00028407152,0.00018613558,0.0056701233],"category_scores_gemma":[0.00012619124,0.00009079166,0.00012751637,0.00039276484,0.0002879979,0.00022126739,0.000105356805,0.0005318122,0.00036171675],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009620616,0.00001922964,0.0012632243,0.00002142498,0.00000559129,0.000042126354,0.000047228437,0.00004807683,0.9935462,0.00026529044,0.00042758338,0.004217938],"study_design_scores_gemma":[0.000017685883,0.000108971886,0.064508736,0.0000064404517,0.00001810474,0.00031115403,0.00007484215,0.0024830122,0.92550224,0.00022102012,0.0067346036,0.000013160002],"about_ca_topic_score_codex":0.003097692,"about_ca_topic_score_gemma":0.004156299,"teacher_disagreement_score":0.0056701233,"about_ca_system_score_codex":0.00037574422,"about_ca_system_score_gemma":0.00012303411,"threshold_uncertainty_score":0.018968463},"labels":[],"label_agreement":null},{"id":"W2163500003","doi":"10.1088/0004-637x/794/2/165","title":"CARMA LARGE AREA STAR FORMATION SURVEY: PROJECT OVERVIEW WITH ANALYSIS OF DENSE GAS STRUCTURE AND KINEMATICS IN BARNARD 1","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"University of Illinois at Urbana-Champaign; California Institute of Technology; Gordon and Betty Moore Foundation; James S. McDonnell Foundation; National Science Foundation","keywords":"Serpens; Protostar; Star formation; Spectral resolution; Molecular cloud; Kinematics; Ridge; Angular resolution (graph drawing)","score_opus":0.017269873335667076,"score_gpt":0.2569712109652586,"score_spread":0.23970133762959153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163500003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83249444,0.010169954,0.009798045,0.0017485637,0.00008108446,0.0020204412,0.10375579,0.002030199,0.037901435],"genre_scores_gemma":[0.7692435,0.0044114674,0.050200596,0.0008004806,0.00030061914,0.0015380068,0.15544665,0.0004060625,0.017652754],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99964976,0.00004964658,0.00000960096,0.00009037991,0.00012782431,0.00007271239],"domain_scores_gemma":[0.9992187,0.000044613636,0.0001600868,0.00008071093,0.00024821414,0.00024762683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007237894,0.00037646163,0.00029511718,0.0042106565,0.000499057,0.00053533056,0.0008966812,0.00031074646,0.003033797],"category_scores_gemma":[0.00064648694,0.00021991941,0.0001844021,0.0023025845,0.0001325845,0.00041445773,0.0011039417,0.00022955179,0.0013468375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035181764,0.0003525606,0.7464773,0.00036811462,0.0001337628,0.00025542983,0.0007528903,0.0015309226,0.010338898,0.0009344006,0.05615929,0.18234466],"study_design_scores_gemma":[0.000025034702,0.00008284621,0.94166607,0.000034925044,0.000019697733,0.00014806842,0.00019910443,0.0009722263,0.00086155464,0.00009749119,0.05587963,0.000013460027],"about_ca_topic_score_codex":0.08279774,"about_ca_topic_score_gemma":0.107456475,"teacher_disagreement_score":0.08279774,"about_ca_system_score_codex":0.001126751,"about_ca_system_score_gemma":0.0010632682,"threshold_uncertainty_score":0.1646316},"labels":[],"label_agreement":null},{"id":"W2163547226","doi":"10.1088/0004-637x/785/2/134","title":"REIONIZATION HISTORIES OF MILKY WAY MASS HALOS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Reionization; Halo; Redshift; Dark matter; Milky Way; Galaxy; Cosmology; Dark Ages","score_opus":0.005632352129067294,"score_gpt":0.1906288164478339,"score_spread":0.1849964643187666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163547226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980426,0.00018707817,0.00012468858,0.000020136173,0.000001670678,0.0000034429193,0.00039028944,0.000025745621,0.0012044166],"genre_scores_gemma":[0.99751437,0.000051323103,0.000059491736,0.000010135024,0.0000017552791,0.0000025153836,0.0006413204,0.000021376723,0.0016977652],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999186,0.0000061320748,0.0000026840655,0.000016571941,0.000015547688,0.000040527237],"domain_scores_gemma":[0.999252,0.00015161773,0.00015952108,0.00010875654,0.000120933815,0.00020713847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003362026,0.00018363919,0.00024857352,0.0014554828,0.00039326728,0.0006494017,0.00035452153,0.00024778367,0.0038564862],"category_scores_gemma":[0.0012131539,0.00017141049,0.00035333616,0.0007039346,0.00020958914,0.00040929642,0.0009149933,0.00023570147,0.0006490997],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012175168,0.00011199076,0.8502091,0.000100761084,0.00041686668,0.0011965554,0.0016735222,0.021998473,0.08927495,0.0019402518,0.0015773729,0.030282615],"study_design_scores_gemma":[0.000015903233,0.000084582556,0.98183113,0.000012899543,0.000057563404,0.00022944476,0.0004032294,0.0054299473,0.008859823,0.00050349167,0.0025393297,0.000032623037],"about_ca_topic_score_codex":0.008421208,"about_ca_topic_score_gemma":0.006293784,"teacher_disagreement_score":0.008421208,"about_ca_system_score_codex":0.0007671608,"about_ca_system_score_gemma":0.0001438659,"threshold_uncertainty_score":0.016744375},"labels":[],"label_agreement":null},{"id":"W2163555909","doi":"10.1088/0004-637x/730/2/72","title":"CARMA SURVEY TOWARD INFRARED-BRIGHT NEARBY GALAXIES (STING): MOLECULAR GAS STAR FORMATION LAW IN NGC 4254","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Astrophysics; Surface brightness; Star formation; Extinction (optical mineralogy); Infrared; Physics; Galaxy; Brightness; TRACER; Astronomy; Optics","score_opus":0.024458193740674525,"score_gpt":0.2357724352564739,"score_spread":0.21131424151579936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163555909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904865,0.00004955232,0.00021870223,0.000011193897,0.0000010005024,0.0000043571563,0.00016010489,0.000028891793,0.00047753248],"genre_scores_gemma":[0.9985837,0.000028534281,0.0006380626,0.000011285704,0.0000024007875,0.0000059323465,0.00045690825,0.000005755533,0.0002674872],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979407,0.00003664556,0.000009159024,0.00007006403,0.00005577655,0.0000342513],"domain_scores_gemma":[0.9996013,0.00005564297,0.00011673087,0.00006598459,0.00007450356,0.00008585364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004346013,0.00019661298,0.00021406096,0.0009104867,0.00033681345,0.00038450753,0.00048309856,0.00022669836,0.00071843463],"category_scores_gemma":[0.0009037464,0.00015360018,0.00017515101,0.0005631582,0.00021067867,0.00020194123,0.00043269043,0.00015311207,0.00020224298],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017858007,0.00007048434,0.97118896,0.000030297942,0.00007654257,0.00023951412,0.00057022285,0.001522493,0.017304169,0.00021831022,0.00035116312,0.008249292],"study_design_scores_gemma":[0.000005068879,0.000019084377,0.99680233,0.0000036856381,0.000018476901,0.000060543516,0.00010971435,0.0020937982,0.0004933025,0.000022267575,0.00036814317,0.0000036010501],"about_ca_topic_score_codex":0.06075438,"about_ca_topic_score_gemma":0.11921581,"teacher_disagreement_score":0.06075438,"about_ca_system_score_codex":0.00062523433,"about_ca_system_score_gemma":0.0003296822,"threshold_uncertainty_score":0.12080151},"labels":[],"label_agreement":null},{"id":"W2163812193","doi":"10.1088/0004-637x/743/2/114","title":"Pan-STARRS1 DISCOVERY OF TWO ULTRALUMINOUS SUPERNOVAE AT<i>z</i>≈ 0.9","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":203,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Max-Planck-Gesellschaft; Ministerio de Ciencia, Tecnología e Innovación Productiva; Queen's University Belfast; Queen's University; University of Edinburgh; Johns Hopkins University; National Radio Astronomy Observatory; Harvard University; Durham University; Smithsonian Institution; Ministério da Ciência e Tecnologia; National Science Foundation","keywords":"Supernova; Physics; Astrophysics; Light curve; Magnetar; Rest frame; Spectral line; Spectroscopy; Astronomy; Galaxy; Redshift; Neutron star","score_opus":0.018172104901937516,"score_gpt":0.2296740277645172,"score_spread":0.21150192286257968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2163812193","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961008,0.00034287476,0.0004641277,0.00005229614,0.000009456789,0.0000092462715,0.0004060278,0.000050834664,0.0025643217],"genre_scores_gemma":[0.99642086,0.00030575876,0.00092192215,0.000050527884,0.000016831667,0.000006620482,0.0014291095,0.0000115333505,0.0008368132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998548,0.000011709271,0.000008093529,0.000045773362,0.000046735044,0.00003287064],"domain_scores_gemma":[0.99956244,0.000033179935,0.0001717583,0.00003839964,0.000051439805,0.00014283249],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002961194,0.00030483815,0.00023649384,0.00097064395,0.00033073995,0.0006535389,0.00026211183,0.00026291073,0.0009792835],"category_scores_gemma":[0.00042914387,0.00018598798,0.0002927894,0.00044721528,0.00019479699,0.0003113523,0.0008756062,0.0003308522,0.00028549152],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055949553,0.000054704928,0.85249335,0.00013315481,0.0002033593,0.0014394153,0.00031456156,0.0004445206,0.101339266,0.0015646252,0.001035847,0.040417667],"study_design_scores_gemma":[0.000010857181,0.00015924245,0.9868176,0.000012213787,0.000036637502,0.0015429076,0.00009878409,0.00036678003,0.0046676146,0.00018500003,0.0060935193,0.000008772228],"about_ca_topic_score_codex":0.0016374398,"about_ca_topic_score_gemma":0.0033301772,"teacher_disagreement_score":0.0016374398,"about_ca_system_score_codex":0.00024777398,"about_ca_system_score_gemma":0.00015960513,"threshold_uncertainty_score":0.0032759905},"labels":[],"label_agreement":null},{"id":"W2164320268","doi":"10.1086/321487","title":"Phase‐dependent Spectral Variability in 4U 1907+09","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"High-pressure geophysics and materials","field":"Earth and Planetary Sciences","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; McGill University","funders":"","keywords":"Physics; Astrophysics; Pulsar; Flux (metallurgy); Neutron star; Orbit (dynamics); Sky; Light curve; Spectral line; X-ray binary; Astronomy; Absorption (acoustics); Flare; X-ray pulsar; Optics","score_opus":0.010757701536439922,"score_gpt":0.23008921726224138,"score_spread":0.21933151572580145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2164320268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990427,0.000048107235,0.000091091286,0.000014239619,0.000005107096,0.0000031695079,0.00014230762,0.000010236371,0.0006429664],"genre_scores_gemma":[0.99863964,0.000034457793,0.00017697923,0.000017878307,0.000014184536,0.0000074205677,0.00089021266,0.000008633239,0.00021071834],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999058,0.000012566967,0.0000038456287,0.00002139934,0.000020572481,0.000035792204],"domain_scores_gemma":[0.9997645,0.00003369055,0.00008850801,0.000018751796,0.00005292923,0.000041639272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015038361,0.00016417091,0.00023522641,0.00084188156,0.00041755015,0.00041031683,0.00019543343,0.00022876174,0.0007465346],"category_scores_gemma":[0.00044770792,0.00013020515,0.00011514619,0.00043955873,0.00026694575,0.00016626391,0.0003805832,0.00021822938,0.00028395996],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059086806,0.0002236501,0.9024485,0.000038012447,0.000068968715,0.00046495497,0.0004893932,0.0006159891,0.07166188,0.0005562976,0.0012637762,0.021577766],"study_design_scores_gemma":[0.000013187662,0.00011408449,0.9954928,0.0000034585269,0.00001435558,0.0002997945,0.00007015396,0.0007050757,0.0015515127,0.00008685151,0.0016410286,0.00000768091],"about_ca_topic_score_codex":0.0031070863,"about_ca_topic_score_gemma":0.0060219974,"teacher_disagreement_score":0.0031070863,"about_ca_system_score_codex":0.0002831276,"about_ca_system_score_gemma":0.00011229886,"threshold_uncertainty_score":0.0061780214},"labels":[],"label_agreement":null},{"id":"W2164335046","doi":"10.1086/506254","title":"Polarization Observations of the Anomalous Microwave Emission in the Perseus Molecular Complex with the COSMOSOMAS Experiment","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Polarization (electrochemistry); Dipole; Microwave; Astrophysics; Cosmic microwave background; Atomic physics; Optics; Chemistry","score_opus":0.011194075603433981,"score_gpt":0.21231781430786734,"score_spread":0.20112373870443334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2164335046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951857,0.00007095658,0.0011786261,0.0000603702,0.0000072527987,0.000005472147,0.00039092425,0.000051375217,0.0030494437],"genre_scores_gemma":[0.9978661,0.000046319958,0.0014093015,0.000017905906,0.000009691254,0.000004481406,0.00038547124,0.000012013149,0.000248719],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999864,0.0000275206,0.0000036859747,0.00004147066,0.00003645797,0.000026829914],"domain_scores_gemma":[0.99974066,0.000032816744,0.00006957781,0.00006631175,0.000047998088,0.000042545205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034266454,0.0002519255,0.00015323797,0.00058955565,0.000268216,0.0002753978,0.00015072843,0.0001509436,0.00072890706],"category_scores_gemma":[0.00029089625,0.00015848277,0.00015241477,0.0005240843,0.00037469078,0.00018318885,0.00049331243,0.0002453524,0.00012922035],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022263478,0.000112458525,0.23552462,0.00006577295,0.0002128874,0.0009861958,0.00048122002,0.0032116433,0.72619295,0.0046129217,0.001902841,0.024470111],"study_design_scores_gemma":[0.0003604366,0.0002635487,0.8036771,0.000020259049,0.00014248415,0.0010766191,0.00019138299,0.0067248093,0.17682482,0.0017476953,0.008926156,0.000044686418],"about_ca_topic_score_codex":0.0012763378,"about_ca_topic_score_gemma":0.002012559,"teacher_disagreement_score":0.0012763378,"about_ca_system_score_codex":0.00022316304,"about_ca_system_score_gemma":0.00011384022,"threshold_uncertainty_score":0.002537787},"labels":[],"label_agreement":null},{"id":"W2164849052","doi":"10.1088/0004-637x/742/1/13","title":"THE FIRST MASSIVE BLACK HOLE SEEDS AND THEIR HOSTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Black hole (networking); Stellar black hole; Intermediate-mass black hole; Binary black hole; Halo; Primordial black hole; Spin-flip","score_opus":0.008577605525965454,"score_gpt":0.19018611201290025,"score_spread":0.1816085064869348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2164849052","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974366,0.0000845088,0.0013903286,0.000055440778,0.000003055778,0.000005474073,0.00003484349,0.000028401324,0.000961326],"genre_scores_gemma":[0.9993637,0.0000305631,0.00037961523,0.000008746427,0.0000019052507,0.0000022749496,0.000029753777,0.0000074333666,0.00017602147],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990785,0.000017840408,0.0000026843388,0.000021156611,0.000015215562,0.000035093464],"domain_scores_gemma":[0.9988212,0.00028447196,0.0003369809,0.00008127036,0.00006694164,0.00040915058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049388385,0.00031047166,0.0003615368,0.0004153552,0.0005006307,0.000996294,0.00041427958,0.0004943786,0.0013309771],"category_scores_gemma":[0.0027380486,0.00031228873,0.00030755566,0.00019567937,0.0007078926,0.00085321604,0.0008587832,0.00043887168,0.0002031773],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007276066,0.00025403523,0.49357992,0.00016415343,0.00023039883,0.0016244327,0.0010797207,0.3883759,0.045738302,0.053373378,0.0017352591,0.013116912],"study_design_scores_gemma":[0.00033900086,0.0004531907,0.18867706,0.000051262687,0.00012012218,0.0006030031,0.00071340986,0.76608294,0.01712692,0.022684252,0.0030661041,0.00008268586],"about_ca_topic_score_codex":0.003882027,"about_ca_topic_score_gemma":0.0027736009,"teacher_disagreement_score":0.003882027,"about_ca_system_score_codex":0.00064873265,"about_ca_system_score_gemma":0.00031926416,"threshold_uncertainty_score":0.007718861},"labels":[],"label_agreement":null},{"id":"W2164905520","doi":"10.1088/0004-637x/767/1/34","title":"OBSERVATIONS OF INTENSITY FLUCTUATIONS ATTRIBUTED TO GRANULATION AND FACULAE ON SUN-LIKE STARS FROM THE<i>KEPLER</i>MISSION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Stars; Granulation; Spectral line; Intensity (physics); Variable star; Frequency spectrum; Spectrum analysis","score_opus":0.03065767233221482,"score_gpt":0.23998530763684697,"score_spread":0.20932763530463216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2164905520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990552,0.00005251797,0.0002887266,0.000007218863,0.0000017677061,0.000005014405,0.0002476879,0.000025476545,0.00031628384],"genre_scores_gemma":[0.99839634,0.000045904784,0.0006059614,0.0000065082745,0.000009819987,0.000004844197,0.00079414155,0.000015865404,0.000120572746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998549,0.000014712345,0.000013059673,0.00004094522,0.000044692435,0.000031638323],"domain_scores_gemma":[0.9993579,0.00010768249,0.00027179555,0.000058250112,0.00009044421,0.00011405798],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030112665,0.00023051024,0.00025401832,0.0015866525,0.00031919326,0.00034999402,0.00022831393,0.0003151904,0.0005416584],"category_scores_gemma":[0.0005935124,0.00018378475,0.00025818238,0.0010265225,0.00026663468,0.000253251,0.00036481014,0.00026494396,0.00018154943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006748572,0.000119587974,0.84678894,0.00007807042,0.00016951263,0.000581063,0.00070042536,0.0013999045,0.13519065,0.00012029029,0.0003472617,0.013829348],"study_design_scores_gemma":[0.0000042195957,0.00003112814,0.9962366,0.0000019429704,0.0000123217615,0.00016342661,0.000028947816,0.0005488209,0.0027635826,0.000015296937,0.00018986895,0.0000038710773],"about_ca_topic_score_codex":0.0017227927,"about_ca_topic_score_gemma":0.0031642655,"teacher_disagreement_score":0.0017227927,"about_ca_system_score_codex":0.00026342913,"about_ca_system_score_gemma":0.000079665864,"threshold_uncertainty_score":0.0034255981},"labels":[],"label_agreement":null},{"id":"W2164948292","doi":"10.1086/498335","title":"Arecibo Pulsar Survey Using ALFA. I. Survey Strategy and First Discoveries","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":268,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China; Fonds Québécois de la Recherche sur la Nature et les Technologies; Princeton University; National Aeronautics and Space Administration; Goddard Space Flight Center; Universities Space Research Association; National Science Foundation","keywords":"Pulsar; Astronomy; Survey research; Physics; Geology; Remote sensing; Sociology","score_opus":0.021589931847891375,"score_gpt":0.24112388123393375,"score_spread":0.21953394938604237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2164948292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9277423,0.0010706855,0.006788008,0.00041406442,0.000063797575,0.0005151536,0.020833554,0.0010253517,0.04154705],"genre_scores_gemma":[0.87515324,0.0021753567,0.03813551,0.0005019539,0.00022361545,0.0008959567,0.064675234,0.00022762152,0.018011518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997354,0.00003581731,0.000012691506,0.000055728084,0.000110042216,0.000050398972],"domain_scores_gemma":[0.9993229,0.00003418394,0.00013903865,0.00009234735,0.0003160486,0.00009547633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059974904,0.00031354828,0.0002630567,0.0027239164,0.00067143043,0.0005383924,0.00042687164,0.00025680265,0.0012807521],"category_scores_gemma":[0.00051929743,0.00013431533,0.00018984826,0.0020964225,0.00016582804,0.00020542114,0.00043343662,0.00020921257,0.0011216657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010496725,0.00028557895,0.6918735,0.00028642,0.00016886125,0.0007823733,0.0010622676,0.0010459502,0.075363345,0.0011424384,0.023324851,0.20361465],"study_design_scores_gemma":[0.00004901258,0.0001700878,0.9417837,0.000028336888,0.000042486812,0.00025036195,0.00018872882,0.00079014833,0.004581206,0.00012597902,0.051977057,0.00001299409],"about_ca_topic_score_codex":0.03470199,"about_ca_topic_score_gemma":0.05260397,"teacher_disagreement_score":0.03470199,"about_ca_system_score_codex":0.00074530026,"about_ca_system_score_gemma":0.0009350165,"threshold_uncertainty_score":0.069000006},"labels":[],"label_agreement":null},{"id":"W2165134157","doi":"10.1088/0004-637x/775/2/105","title":"<i>KEPLER</i>PLANETS: A TALE OF EVAPORATION","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":771,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Planet; Population; Terrestrial planet; Planetary mass; Evaporation; Kepler; Envelope (radar)","score_opus":0.00916139929690859,"score_gpt":0.24746327194471354,"score_spread":0.23830187264780495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165134157","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17637046,0.1421419,0.102458544,0.14309825,0.0134613,0.00012138005,0.002218187,0.0023679428,0.417762],"genre_scores_gemma":[0.6966637,0.049750425,0.044474594,0.017871821,0.010828257,0.00015472069,0.001003416,0.003080456,0.1761727],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99977666,0.00007868535,0.000010715009,0.00004754577,0.000049300936,0.000037102636],"domain_scores_gemma":[0.99969065,0.00011242801,0.000040369734,0.000063016625,0.00004134225,0.000052123924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005386996,0.00049224216,0.00030472543,0.0009634564,0.001605057,0.0040521147,0.00070131605,0.0011468868,0.006328913],"category_scores_gemma":[0.001538525,0.00029143924,0.0005151628,0.0007781761,0.0035427576,0.0063006408,0.002520314,0.0026685428,0.0014464256],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016517259,0.000034922996,0.007880452,0.00033533145,0.00007720553,0.0012838512,0.006124007,0.0069109504,0.004997713,0.73711294,0.12820432,0.1068732],"study_design_scores_gemma":[0.0000076261113,0.000054112443,0.010426651,0.0003230095,0.000017495458,0.0015561297,0.0015996698,0.0041349987,0.0013721529,0.32703534,0.65340084,0.00007205774],"about_ca_topic_score_codex":0.0025150904,"about_ca_topic_score_gemma":0.0032689637,"teacher_disagreement_score":0.006328913,"about_ca_system_score_codex":0.001152498,"about_ca_system_score_gemma":0.0003590964,"threshold_uncertainty_score":0.021172345},"labels":[],"label_agreement":null},{"id":"W2165334869","doi":"10.1086/377212","title":"PSR J1847-0130: A Radio Pulsar with Magnetar Spin Characteristics","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"","keywords":"Pulsar; Magnetar; Physics; Neutron star; Astrophysics; X-ray pulsar; Magnetic field; Magnetic dipole; Astronomy; Dipole; Luminosity; Binary pulsar; Field strength; Millisecond pulsar; Galaxy","score_opus":0.008525839078894436,"score_gpt":0.2769732325428438,"score_spread":0.26844739346394936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165334869","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99825114,0.00020741465,0.00022323975,0.00008938694,0.000016366897,0.000008686632,0.00018042389,0.000031462267,0.0009918929],"genre_scores_gemma":[0.99756706,0.0001799915,0.0007111277,0.000089752975,0.000039477472,0.0000062722575,0.00083820976,0.000008159279,0.0005600034],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999224,0.0000067514093,0.000006072367,0.000017726665,0.000023152164,0.000023857747],"domain_scores_gemma":[0.99975437,0.000020679947,0.00010109265,0.000026050639,0.000027734224,0.00007010114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013993664,0.0002576313,0.00022207288,0.00040416175,0.00045338145,0.00042901517,0.00023841257,0.00035127383,0.0006828415],"category_scores_gemma":[0.00026090632,0.00013691606,0.00009084821,0.00048184465,0.00034879756,0.00026139212,0.0005834283,0.00029973206,0.00071055663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005732754,0.00027278054,0.6749321,0.00016557224,0.00007440058,0.0143077625,0.0007484355,0.0006043319,0.26360136,0.0015033968,0.005681051,0.03753552],"study_design_scores_gemma":[0.000110683446,0.0009503998,0.92690706,0.000021764848,0.00005415424,0.029451137,0.00040795378,0.0015342656,0.018442845,0.0013721475,0.020712608,0.00003494254],"about_ca_topic_score_codex":0.0007423094,"about_ca_topic_score_gemma":0.0016351715,"teacher_disagreement_score":0.0007423094,"about_ca_system_score_codex":0.00013275274,"about_ca_system_score_gemma":0.00012656614,"threshold_uncertainty_score":0.0022842884},"labels":[],"label_agreement":null},{"id":"W2165365535","doi":"10.1088/0004-637x/789/2/165","title":"FREQUENCY OF CLOSE COMPANIONS AMONG<i>KEPLER</i>PLANETS—A TRANSIT TIME VARIATION STUDY","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Transit (satellite); Planet; Kepler; Variation (astronomy); Transit time; Planetary system; Exoplanet; Kepler's laws of planetary motion","score_opus":0.00719557305786428,"score_gpt":0.20856585424954355,"score_spread":0.20137028119167927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165365535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995603,0.00004941537,0.00008079136,0.000007207059,6.058713e-7,8.6509743e-7,0.00005655669,0.0000034865689,0.00024066608],"genre_scores_gemma":[0.99978906,0.00001199754,0.00003206085,0.0000011259906,0.0000016486623,3.8903067e-7,0.00010419554,0.0000011422009,0.000058452522],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998103,0.000036987578,0.000016207197,0.00007364471,0.000029923758,0.000033005785],"domain_scores_gemma":[0.9980913,0.0005624367,0.00080487045,0.0001775442,0.00014563775,0.00021815163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026134725,0.000085902626,0.00015138972,0.001236691,0.0003577856,0.00048918143,0.00016850166,0.00022185384,0.0012074312],"category_scores_gemma":[0.0021397704,0.00007518716,0.00014226111,0.0007649146,0.00027532846,0.00042359455,0.0006352185,0.00014649022,0.0002425543],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010209856,0.000012902129,0.9927248,0.00000993332,0.000023846507,0.0001154215,0.00028191635,0.0001920353,0.0023638492,0.00018041216,0.00009078478,0.0039020756],"study_design_scores_gemma":[0.0000024089868,0.00005983487,0.9962846,0.000003231679,0.000017939901,0.00077389885,0.00026357966,0.0012657859,0.0006951416,0.00012459519,0.00050478114,0.0000042370702],"about_ca_topic_score_codex":0.0015350949,"about_ca_topic_score_gemma":0.001864991,"teacher_disagreement_score":0.0015350949,"about_ca_system_score_codex":0.0001789614,"about_ca_system_score_gemma":0.00007784037,"threshold_uncertainty_score":0.0040392876},"labels":[],"label_agreement":null},{"id":"W2165425276","doi":"10.1088/0004-637x/786/1/39","title":"V1309 Sco—UNDERSTANDING A MERGER","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Common envelope; Angular momentum; Orbital period; Binary number; Envelope (radar); Binary star; Star (game theory); Radiative transfer; Event (particle physics)","score_opus":0.020189283421838178,"score_gpt":0.23394022411948506,"score_spread":0.21375094069764689,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165425276","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9688074,0.0021392792,0.008266788,0.0009306023,0.00003057134,0.000027350994,0.00020558388,0.00014476171,0.019447608],"genre_scores_gemma":[0.9954283,0.00089209224,0.0029218472,0.000091134265,0.00003115395,0.000006930481,0.00012851808,0.00003149531,0.00046840264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994504,0.000007834475,0.0000027109995,0.000015143094,0.00001579685,0.000013320942],"domain_scores_gemma":[0.99985886,0.00002869228,0.000047386126,0.000013755092,0.000016828775,0.00003438237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016030703,0.00026037256,0.00029195624,0.00039101014,0.0004955515,0.0013880612,0.00042189934,0.0007192183,0.000622874],"category_scores_gemma":[0.0007710816,0.00018830178,0.00019322496,0.0003375154,0.00060158793,0.0022910219,0.0009026367,0.000597746,0.00017259065],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093053846,0.00026149728,0.3607068,0.0009723013,0.00021792851,0.0040720645,0.006385776,0.08418894,0.23205346,0.19261594,0.008773032,0.10882175],"study_design_scores_gemma":[0.0000573785,0.0004592533,0.49080175,0.00031847306,0.00012188933,0.0025495964,0.0048856945,0.2969808,0.011436179,0.15653585,0.03572876,0.00012435207],"about_ca_topic_score_codex":0.00499791,"about_ca_topic_score_gemma":0.0027835593,"teacher_disagreement_score":0.00499791,"about_ca_system_score_codex":0.0006483818,"about_ca_system_score_gemma":0.00034683128,"threshold_uncertainty_score":0.009937644},"labels":[],"label_agreement":null},{"id":"W2165603825","doi":"10.1088/0004-637x/786/1/76","title":"ERRATUM: “ON THE MASS RADIATED BY COALESCING BLACK-HOLE BINARIES” (ApJ, 2012, 758, 63)","year":2014,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph","funders":"","keywords":"Physics; Astrophysics; Astronomy","score_opus":0.006903064974571499,"score_gpt":0.2021530835152624,"score_spread":0.1952500185406909,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165603825","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.004545908,0.009901012,0.01143949,0.059240624,0.8789984,0.000089373236,0.0034329272,0.0010768942,0.03127543],"genre_scores_gemma":[0.08571609,0.02092358,0.044684414,0.07815174,0.16108334,0.00034049,0.009500935,0.0036441237,0.5959553],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9993061,0.00011168462,0.00009398628,0.00013612896,0.00031003632,0.00004197542],"domain_scores_gemma":[0.99710685,0.00081834313,0.00023504088,0.00022243948,0.0014780728,0.00013929096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012847027,0.0017069636,0.0007499433,0.0023855339,0.0015513026,0.0016204648,0.0023763268,0.0023551178,0.017759226],"category_scores_gemma":[0.010397932,0.0004802961,0.0008224549,0.0015007134,0.0016238193,0.0022387998,0.0011749179,0.0031036246,0.01295259],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007598057,0.000020713378,0.0004606317,0.00016270301,0.000022021073,0.0002525951,0.000048644077,0.00046831105,0.00044505333,0.006487754,0.9733193,0.018236382],"study_design_scores_gemma":[0.000056490906,0.000073433504,0.0062198257,0.0003674945,0.00008404127,0.0006682719,0.00015077637,0.0048752744,0.0022694801,0.011507392,0.97362864,0.00009895477],"about_ca_topic_score_codex":0.016325833,"about_ca_topic_score_gemma":0.016445823,"teacher_disagreement_score":0.017759226,"about_ca_system_score_codex":0.0022423794,"about_ca_system_score_gemma":0.0012287637,"threshold_uncertainty_score":0.059410572},"labels":[],"label_agreement":null},{"id":"W2165640657","doi":"10.3847/0004-637x/818/2/178","title":"SPECTRUM AND ANISOTROPY OF TURBULENCE FROM MULTI-FREQUENCY MEASUREMENT OF SYNCHROTRON POLARIZATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Faraday effect; Synchrotron; Polarization (electrochemistry); Anisotropy; Turbulence; Magnetic field; LOFAR; Synchrotron radiation","score_opus":0.011027816577555912,"score_gpt":0.2080570094343021,"score_spread":0.1970291928567462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165640657","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95486987,0.00007252048,0.043924697,0.00006765786,0.000007639324,0.0000062323006,0.00018042233,0.00007942622,0.0007916246],"genre_scores_gemma":[0.9961898,0.000046095178,0.0035622295,0.0000056008225,0.000011141584,0.0000038353,0.00011105151,0.000008050799,0.000062220446],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998827,0.00003897516,0.0000069238536,0.000019352132,0.00003185726,0.00002026781],"domain_scores_gemma":[0.9991074,0.00043030674,0.00024757447,0.000106779116,0.00006718283,0.000040670453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055769796,0.00030921237,0.0001956887,0.0011746024,0.00018025353,0.00049281726,0.0001909595,0.00020874073,0.00036287794],"category_scores_gemma":[0.0018363897,0.00014009593,0.00020993053,0.00060693204,0.0005798546,0.0006983116,0.0002696745,0.00028822478,0.000051955987],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062993064,0.00024472616,0.15420106,0.00019661139,0.00022888203,0.0008005229,0.0003976277,0.5074359,0.23192443,0.044150196,0.0008853598,0.058904722],"study_design_scores_gemma":[0.000013758015,0.000054289805,0.10883634,0.000012387262,0.000026168596,0.00018940891,0.00006611119,0.87271446,0.011336911,0.0064854436,0.00022543696,0.000039312312],"about_ca_topic_score_codex":0.00092706695,"about_ca_topic_score_gemma":0.0008207009,"teacher_disagreement_score":0.0011746024,"about_ca_system_score_codex":0.0002497749,"about_ca_system_score_gemma":0.00014300316,"threshold_uncertainty_score":0.002949357},"labels":[],"label_agreement":null},{"id":"W2165842865","doi":"10.1088/0004-637x/753/2/134","title":"A COMPREHENSIVE VIEW OF A STRONGLY LENSED<i>PLANCK</i>-ASSOCIATED SUBMILLIMETER GALAXY","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Submillimeter Array; Gravitational lens; Galactic astronomy; Stars; Milky Way; Terahertz radiation; Planck; Extragalactic astronomy","score_opus":0.013736243242522036,"score_gpt":0.2240084280266904,"score_spread":0.21027218478416837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165842865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75916785,0.0097431475,0.012819187,0.0013755269,0.00013073829,0.00008292949,0.04844448,0.004937213,0.16329889],"genre_scores_gemma":[0.95229745,0.004502673,0.0123655,0.00054577744,0.00015548858,0.000048724476,0.021375407,0.00028215258,0.008426875],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995935,0.0000021807875,0.0000012487193,0.000011593132,0.0000102871,0.000015408901],"domain_scores_gemma":[0.9999194,0.0000059792205,0.00002396101,0.000015618843,0.000009077903,0.000025993859],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004512237,0.00030091888,0.00014472127,0.0014794243,0.00028206283,0.0006208222,0.00028274726,0.00021309145,0.0065494804],"category_scores_gemma":[0.00009658299,0.0001941554,0.00027331512,0.0015730553,0.00016040169,0.0004344959,0.00062928966,0.00025996251,0.0020111173],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036906873,0.00016124555,0.36252916,0.0011837198,0.000554906,0.0020407331,0.0021908185,0.008558646,0.2295202,0.010608039,0.102789514,0.27949393],"study_design_scores_gemma":[0.000006707553,0.00003491422,0.885727,0.000034407232,0.000048531183,0.00060923956,0.00020704554,0.0016773537,0.0024481043,0.000874236,0.10831145,0.000020940974],"about_ca_topic_score_codex":0.006464154,"about_ca_topic_score_gemma":0.009360354,"teacher_disagreement_score":0.0065494804,"about_ca_system_score_codex":0.0003533222,"about_ca_system_score_gemma":0.00019753033,"threshold_uncertainty_score":0.02191019},"labels":[],"label_agreement":null},{"id":"W2165885467","doi":"10.1086/512067","title":"Gravitational Recoil Velocities from Eccentric Binary Black Hole Mergers","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph","funders":"","keywords":"Recoil; Binary black hole; Supermassive black hole; Gravitational wave; Stellar black hole; Black hole (networking); Galaxy; Intermediate-mass black hole","score_opus":0.013753880707582603,"score_gpt":0.30086189164255417,"score_spread":0.28710801093497157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165885467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9733499,0.0025139698,0.0121640125,0.00027415802,0.000041348154,0.000013328642,0.00033209904,0.00028856154,0.011022605],"genre_scores_gemma":[0.99834836,0.00037157908,0.0007359887,0.000015822185,0.000015538413,0.000006539305,0.00023401689,0.000037695718,0.00023447417],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99958473,0.00006975637,0.000023915056,0.00008793475,0.00010373882,0.00012981694],"domain_scores_gemma":[0.99539775,0.0026692932,0.0012849243,0.00026658882,0.00020080908,0.0001806514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010825106,0.0006894594,0.00046138195,0.0024296413,0.0005494792,0.0010867149,0.00073807716,0.0007243027,0.0012868991],"category_scores_gemma":[0.0091234725,0.00052965234,0.00034471956,0.0014585069,0.0009878705,0.0011052777,0.0018929545,0.00074962643,0.0003599963],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0035560597,0.00025819012,0.19243434,0.0007078867,0.0002317468,0.0032527621,0.0017360825,0.5441013,0.08919415,0.08555069,0.00324631,0.07573053],"study_design_scores_gemma":[0.00025042915,0.0005870435,0.2640061,0.00028664674,0.00013892722,0.0020583617,0.0005030197,0.5819719,0.090011604,0.054075103,0.0057143103,0.00039654813],"about_ca_topic_score_codex":0.001129061,"about_ca_topic_score_gemma":0.0006565283,"teacher_disagreement_score":0.0024296413,"about_ca_system_score_codex":0.00083587685,"about_ca_system_score_gemma":0.00019312365,"threshold_uncertainty_score":0.0060647726},"labels":[],"label_agreement":null},{"id":"W2165941465","doi":"10.1088/0004-637x/804/1/31","title":"THE<i>HUBBLE</i>WIDE FIELD CAMERA 3 TEST OF SURFACES IN THE OUTER SOLAR SYSTEM: SPECTRAL VARIATION ON KUIPER BELT OBJECTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Photometry (optics); Physics; Astrophysics; Limiting magnitude; Astronomy; Stellar classification; Magnitude (astronomy); Point spread function; Optics; Stars","score_opus":0.00946710328801828,"score_gpt":0.20976737996720146,"score_spread":0.20030027667918318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165941465","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965964,0.00004560492,0.00074041955,0.000018552073,0.0000058832748,0.000012666602,0.00079277443,0.00007342926,0.0017142456],"genre_scores_gemma":[0.996678,0.000021090204,0.0011187844,0.000020124604,0.00000843027,0.000009552829,0.0017735064,0.00003590296,0.00033464708],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998524,0.000010714206,0.000006454272,0.000029628838,0.000060063638,0.000040724077],"domain_scores_gemma":[0.99953973,0.000042119627,0.00014120806,0.000069321446,0.000080092905,0.00012757523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021345381,0.00022365103,0.00021301182,0.0009983378,0.00040278136,0.00052382087,0.00023278002,0.00024664428,0.0010224461],"category_scores_gemma":[0.00033743193,0.000080289574,0.00030323723,0.0007459661,0.00025356218,0.00024843373,0.000341344,0.00032734266,0.00029009473],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043093116,0.00014134237,0.8902765,0.00004371018,0.00010626129,0.00029786088,0.0005018119,0.0012286901,0.08199991,0.00022490452,0.001675371,0.023072744],"study_design_scores_gemma":[0.000003826892,0.00002103994,0.9965431,0.0000013583973,0.0000072626567,0.000062143285,0.0000476645,0.00045240525,0.002439102,0.00002971882,0.00038902575,0.0000032752723],"about_ca_topic_score_codex":0.011188889,"about_ca_topic_score_gemma":0.02481586,"teacher_disagreement_score":0.011188889,"about_ca_system_score_codex":0.00031227712,"about_ca_system_score_gemma":0.00018209885,"threshold_uncertainty_score":0.022247553},"labels":[],"label_agreement":null},{"id":"W2165966273","doi":"10.1086/308561","title":"Combined Analysis of the Binary Lens Caustic‐crossing Event MACHO 98‐SMC‐1","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Gravitational microlensing; Physics; Astrophysics; Binary number; Lens (geology); RADIUS; Caustic (mathematics); Mass ratio; Einstein radius; Limb darkening; Small Magellanic Cloud; Wavelength; Stars; Gravitational lens; Optics; Mathematics; Galaxy","score_opus":0.010594445827648707,"score_gpt":0.23472444871040485,"score_spread":0.22413000288275614,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2165966273","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976412,0.00012348132,0.00041210366,0.000023063445,0.0000058493256,0.000007859756,0.0005831555,0.00006095526,0.0011422825],"genre_scores_gemma":[0.99314815,0.000053032483,0.0010465443,0.000014198028,0.000012848925,0.0000098841165,0.005276846,0.000038436006,0.00040005907],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995372,0.00006998233,0.00002586323,0.00011672507,0.00015268309,0.00009753628],"domain_scores_gemma":[0.9983791,0.00033893998,0.00060549116,0.0001514844,0.00025521498,0.00026985627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007817295,0.00037251745,0.00074518204,0.0018958973,0.00043960064,0.0009513095,0.0004632456,0.0005974088,0.0010570261],"category_scores_gemma":[0.0019141493,0.00026459002,0.0007514585,0.0016326935,0.00017274311,0.00032535332,0.00082003715,0.0003597474,0.00039283957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015843404,0.00029791053,0.9184133,0.0001529955,0.0010273352,0.0012927385,0.0005449519,0.015523497,0.029383294,0.0009986736,0.0019019195,0.028879095],"study_design_scores_gemma":[0.000040877523,0.00012972786,0.9684532,0.000010025831,0.00018834439,0.00033358953,0.0001657227,0.024547534,0.0036474348,0.00025503954,0.0022013888,0.000027149685],"about_ca_topic_score_codex":0.0054262048,"about_ca_topic_score_gemma":0.011522973,"teacher_disagreement_score":0.0054262048,"about_ca_system_score_codex":0.0005783034,"about_ca_system_score_gemma":0.00021230153,"threshold_uncertainty_score":0.010789216},"labels":[],"label_agreement":null},{"id":"W2166195449","doi":"10.1088/0004-637x/785/1/30","title":"THE HARD X-RAY PERSPECTIVE ON THE SOFT X-RAY EXCESS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Accretion (finance); Reflection (computer programming); Active galactic nucleus; Spectral line; Astronomy; Galaxy; Computer science","score_opus":0.013726950538853169,"score_gpt":0.23849148286679717,"score_spread":0.224764532327944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2166195449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9549156,0.0012009073,0.019347558,0.0006481292,0.000042591677,0.000038873175,0.0008772817,0.00027032476,0.022658875],"genre_scores_gemma":[0.99330294,0.00053358503,0.0036137325,0.00011987839,0.000027696418,0.000018005327,0.00031218494,0.00008908562,0.00198292],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99976546,0.00007672795,0.000008073396,0.00006513332,0.00005195724,0.000032613014],"domain_scores_gemma":[0.9988852,0.00057801,0.00016304586,0.00017875501,0.00007268325,0.00012238116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005695012,0.0005469504,0.00051687105,0.0004962788,0.0004206456,0.0021296123,0.000638421,0.0005990446,0.006258021],"category_scores_gemma":[0.002335218,0.0002708358,0.00065541425,0.00042967,0.0010094556,0.0017878421,0.001119511,0.0010978554,0.0008079177],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007761144,0.00012776116,0.25119695,0.00037257417,0.0002969655,0.0010593294,0.0007575351,0.6128202,0.0175281,0.07944084,0.0023136095,0.03331001],"study_design_scores_gemma":[0.00014028899,0.0005917127,0.2393975,0.00023934663,0.00024438664,0.00078560953,0.0008144893,0.6656973,0.007340467,0.07079393,0.013838073,0.000116912066],"about_ca_topic_score_codex":0.0035604327,"about_ca_topic_score_gemma":0.002675238,"teacher_disagreement_score":0.006258021,"about_ca_system_score_codex":0.00046827694,"about_ca_system_score_gemma":0.0002898611,"threshold_uncertainty_score":0.020935118},"labels":[],"label_agreement":null},{"id":"W2166526166","doi":"10.1088/0004-637x/815/1/68","title":"STAR CLUSTER FORMATION WITH STELLAR FEEDBACK AND LARGE-SCALE INFLOW","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Serpens; Accretion (finance); Cluster (spacecraft); Radiation pressure; Stars; Star cluster; Stellar mass; Protostar; Star formation","score_opus":0.010234756536367198,"score_gpt":0.21971984768802716,"score_spread":0.20948509115165997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2166526166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98430276,0.00014370497,0.00954016,0.00014848047,0.000020630529,0.00003345904,0.000099882054,0.00017243411,0.0055384953],"genre_scores_gemma":[0.99843365,0.000056388842,0.0005327231,0.000012863757,0.000006005146,0.000006881232,0.000026034715,0.000010545211,0.00091491523],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986124,0.000028232515,0.000008285681,0.00004301772,0.000018664274,0.000040405357],"domain_scores_gemma":[0.9993839,0.00011919698,0.00021669833,0.000052288386,0.00004434066,0.00018356534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031407844,0.0006824242,0.00047681393,0.0002859372,0.0005346439,0.0012324877,0.0008548391,0.0007482753,0.001642668],"category_scores_gemma":[0.0014443953,0.00030051605,0.00052970665,0.00028548637,0.0010035349,0.00082724786,0.00079613796,0.00026896578,0.00033135666],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036920502,0.00019690972,0.11869114,0.000106899,0.00010459672,0.00090564205,0.0003551433,0.82778186,0.009506027,0.035961367,0.0006879234,0.0053333184],"study_design_scores_gemma":[0.0002745345,0.0003461527,0.04053945,0.000018199045,0.000087804605,0.0003481424,0.00020056855,0.9354761,0.001735513,0.019622715,0.001309896,0.000040959374],"about_ca_topic_score_codex":0.019030321,"about_ca_topic_score_gemma":0.010342112,"teacher_disagreement_score":0.019030321,"about_ca_system_score_codex":0.0017269242,"about_ca_system_score_gemma":0.0010245182,"threshold_uncertainty_score":0.037839115},"labels":[],"label_agreement":null},{"id":"W2166531135","doi":"10.1086/319465","title":"NICMOS Observations of Extragalactic Cepheids. I. Photometry Database and a Test of the Standard Extinction Law","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Photometry (optics); Cosmic distance ladder; Galaxy; Hubble space telescope; Hubble sequence; Metallicity","score_opus":0.014764651609559233,"score_gpt":0.22937104782358944,"score_spread":0.21460639621403022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2166531135","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.845342,0.00031923107,0.001263873,0.000110490495,0.000030044015,0.00015348164,0.1340057,0.00034993648,0.018425217],"genre_scores_gemma":[0.6921195,0.00042552958,0.009036658,0.0001204404,0.00004160777,0.00033588373,0.29211217,0.00010304781,0.005705198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99948883,0.0000768155,0.000040104394,0.000107920525,0.00020028041,0.00008598851],"domain_scores_gemma":[0.9985474,0.000097722776,0.00031206847,0.00047243416,0.00041364916,0.00015662261],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052352314,0.00037369409,0.0003538892,0.0020075266,0.00057170296,0.00037730773,0.00047385207,0.00022107802,0.0033759256],"category_scores_gemma":[0.0014986456,0.00013497862,0.0001616993,0.0023691254,0.00014589095,0.00033150453,0.0007697953,0.00021742373,0.0014149036],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012703831,0.00046770144,0.84351826,0.00035328118,0.00020496249,0.0005871795,0.0013961268,0.0050277966,0.014102922,0.0050467122,0.05991712,0.06810752],"study_design_scores_gemma":[0.000033439377,0.00004541804,0.9409116,0.000021579875,0.00003311324,0.00025074417,0.00021427739,0.0029931602,0.0029123125,0.0005082601,0.05206332,0.000012768143],"about_ca_topic_score_codex":0.023248287,"about_ca_topic_score_gemma":0.032589015,"teacher_disagreement_score":0.023248287,"about_ca_system_score_codex":0.00077626377,"about_ca_system_score_gemma":0.00034699118,"threshold_uncertainty_score":0.046225905},"labels":[],"label_agreement":null},{"id":"W2167078400","doi":"10.1086/505385","title":"<i>Chandra</i>Observations of SDSS J1004+4112: Constraints on the Lensing Cluster and Anomalous X‐Ray Flux Ratios of the Quadruply Imaged Quasar","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Gravitational microlensing; Quasar; Gravitational lens; Luminosity; Flux (metallurgy); Cluster (spacecraft); Strong gravitational lensing; Galaxy; Redshift; Chemistry","score_opus":0.010177325835106466,"score_gpt":0.20064072944198855,"score_spread":0.19046340360688208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167078400","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99774194,0.00010979902,0.00020603817,0.000046876536,0.0000034781824,0.0000062228874,0.00068695407,0.000063844076,0.0011349301],"genre_scores_gemma":[0.9946121,0.00011760392,0.0013097469,0.00004165945,0.000020618047,0.000012167583,0.0033047681,0.000021160682,0.0005602683],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998223,0.000016631962,0.000012913629,0.000030493928,0.000053548374,0.00006417862],"domain_scores_gemma":[0.9994388,0.00007082271,0.00019885197,0.00008562415,0.00006696635,0.0001389633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026911995,0.00050949614,0.00026045076,0.0016012113,0.0005522288,0.0009302881,0.00040372452,0.0004001075,0.0013515262],"category_scores_gemma":[0.0007702693,0.00039519262,0.00023557608,0.001065054,0.00037626197,0.00037055716,0.00067120045,0.00031847405,0.0004377117],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014052915,0.000434334,0.7001155,0.00021427247,0.00030027376,0.0014000998,0.00034837532,0.005136295,0.26793587,0.00078220206,0.0035249838,0.018402545],"study_design_scores_gemma":[0.000086362284,0.00010137403,0.9727418,0.000015059313,0.000086554566,0.0010685169,0.00014216332,0.0040323692,0.018247643,0.00038783147,0.003030675,0.0000596418],"about_ca_topic_score_codex":0.006466117,"about_ca_topic_score_gemma":0.015952114,"teacher_disagreement_score":0.006466117,"about_ca_system_score_codex":0.00048403867,"about_ca_system_score_gemma":0.00023251917,"threshold_uncertainty_score":0.01285696},"labels":[],"label_agreement":null},{"id":"W2167281276","doi":"10.1088/0004-637x/774/2/131","title":"A CHANGE IN THE QUIESCENT X-RAY SPECTRUM OF THE NEUTRON STAR LOW-MASS X-RAY BINARY MXB 1659–29","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Neutron star; X-ray binary; Accretion (finance); Binary star; X-ray burster; Binary number; Accretion disc; Flux (metallurgy)","score_opus":0.014459809929794154,"score_gpt":0.22443561143375187,"score_spread":0.20997580150395773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167281276","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99869627,0.00020527687,0.000109296445,0.000038847134,0.000009711256,0.000002995881,0.000109446955,0.00001537861,0.00081278564],"genre_scores_gemma":[0.9991811,0.000058910588,0.00015395654,0.00004051326,0.000010832861,0.0000021445683,0.00023882352,0.0000062406416,0.0003074502],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999399,0.0000054376437,0.00000418255,0.000025901449,0.000011839563,0.00001275086],"domain_scores_gemma":[0.9997627,0.000020724145,0.000096743235,0.000018820629,0.000027540416,0.00007347747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015504032,0.00015427083,0.0002160318,0.00041657628,0.00025231804,0.00050647877,0.0001727156,0.0003173227,0.0007394014],"category_scores_gemma":[0.0003241987,0.00015086589,0.0001301241,0.00019173654,0.00026400568,0.00030456568,0.00028290044,0.00037892535,0.00022208557],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001105919,0.0002128169,0.37749764,0.00017044506,0.000108479595,0.0029657988,0.0008691276,0.0003604212,0.599462,0.00088290195,0.00091246807,0.015451941],"study_design_scores_gemma":[0.000009425577,0.00007435401,0.9941454,0.0000085290585,0.0000135796145,0.0005453691,0.0000769957,0.00038495287,0.0039644507,0.00007514464,0.0006946612,0.000007024576],"about_ca_topic_score_codex":0.0015798212,"about_ca_topic_score_gemma":0.0019812048,"teacher_disagreement_score":0.0015798212,"about_ca_system_score_codex":0.0002299838,"about_ca_system_score_gemma":0.000077430894,"threshold_uncertainty_score":0.0031412244},"labels":[],"label_agreement":null},{"id":"W2167515605","doi":"10.1088/0004-637x/800/2/123","title":"TIMING OF FIVE MILLISECOND PULSARS DISCOVERED IN THE PALFA SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Canada Research Chairs; Compute Canada; Fonds Québécois de la Recherche sur la Nature et les Technologies; McGill University; Canadian Institute for Advanced Research; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Science Foundation","keywords":"Millisecond pulsar; Millisecond; Pulsar; Astrophysics; Astronomy; Physics","score_opus":0.04416044515750416,"score_gpt":0.3449875605907421,"score_spread":0.3008271154332379,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167515605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98764056,0.0008820348,0.0003160886,0.00026933322,0.000049516817,0.000019397872,0.004364511,0.00006918276,0.0063893506],"genre_scores_gemma":[0.9921828,0.00051694765,0.0003959419,0.000048210946,0.00004353972,0.000019563073,0.00485667,0.0000150995365,0.0019212494],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998204,0.000014151892,0.000019873438,0.000045101715,0.000058210197,0.000042281226],"domain_scores_gemma":[0.99804366,0.00028910098,0.0008749464,0.000084727,0.0004221094,0.0002854752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034912524,0.00014810091,0.00018704489,0.0033765,0.00040193388,0.0006204211,0.00023643814,0.00023781887,0.0023706045],"category_scores_gemma":[0.001465311,0.00012495469,0.0001427993,0.0013088662,0.00020051873,0.00036557709,0.0010857593,0.00031242752,0.0005264851],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004936397,0.000040278075,0.95250297,0.00009431796,0.000097548786,0.00042653666,0.0009525487,0.00021734682,0.0059197824,0.00086121034,0.004494407,0.033899322],"study_design_scores_gemma":[0.0000042710913,0.000032483502,0.99640036,0.000008230012,0.00000770675,0.00015158553,0.00014741915,0.00005150827,0.00021397424,0.000025833673,0.002953688,0.000003001365],"about_ca_topic_score_codex":0.007425058,"about_ca_topic_score_gemma":0.014206558,"teacher_disagreement_score":0.007425058,"about_ca_system_score_codex":0.00041173564,"about_ca_system_score_gemma":0.0002862858,"threshold_uncertainty_score":0.014763713},"labels":[],"label_agreement":null},{"id":"W2167553143","doi":"10.1086/588213","title":"<i>XMM‐Newton</i>Observations of the Narrow‐Line Seyfert 1 Galaxy Mrk 335 in a Historical Low X‐Ray Flux State","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Galaxy; Flux (metallurgy); Emission spectrum; Spectroscopy; Spectral line; Ionization; Line (geometry); Light curve","score_opus":0.020901572934451346,"score_gpt":0.21663197714048754,"score_spread":0.19573040420603618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167553143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981743,0.000259469,0.00014627558,0.000071723065,0.0000061848577,0.000003495008,0.00036627773,0.00004684866,0.0009255645],"genre_scores_gemma":[0.99792296,0.00013668062,0.0005614807,0.00003381147,0.000025742755,0.0000028237785,0.0007574754,0.0000074258146,0.0005517884],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994993,0.00000319425,0.0000036013657,0.0000128023585,0.000019073439,0.00001144277],"domain_scores_gemma":[0.9997892,0.000009185517,0.0001216036,0.000022064647,0.000021003654,0.00003702788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015525408,0.00017191625,0.00015270572,0.00074725423,0.00033006776,0.00036423712,0.00020845055,0.00027453448,0.0010022636],"category_scores_gemma":[0.00020563787,0.00009469674,0.00011690729,0.0004053834,0.00020217165,0.00026464654,0.00029868144,0.00026543747,0.00036003377],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053811626,0.00016145673,0.82960045,0.00013729208,0.0001361925,0.0020980232,0.0009396332,0.00050195557,0.13592942,0.00043348223,0.003426216,0.026097711],"study_design_scores_gemma":[0.000003997869,0.00007041505,0.99473864,0.0000064054266,0.00002350254,0.0005567313,0.00006989947,0.00017551305,0.0019749464,0.00003425922,0.0023401852,0.0000054462143],"about_ca_topic_score_codex":0.0024383317,"about_ca_topic_score_gemma":0.0076390137,"teacher_disagreement_score":0.0024383317,"about_ca_system_score_codex":0.00022700636,"about_ca_system_score_gemma":0.00007369619,"threshold_uncertainty_score":0.004848242},"labels":[],"label_agreement":null},{"id":"W2167597841","doi":"10.1088/0004-637x/738/2/169","title":"MULTIWAVELENGTH OBSERVATIONS OF THE VERY HIGH ENERGY BLAZAR 1ES 2344+514","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Crab Nebula; Blazar; BL Lac object; Flare; Flux (metallurgy); Photon; Gamma ray; Extragalactic background light","score_opus":0.01970190382142431,"score_gpt":0.19521559168672203,"score_spread":0.17551368786529772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167597841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9918637,0.00015604381,0.00037925685,0.000055986922,0.000014488668,0.000024345658,0.0012782365,0.00011523125,0.006112562],"genre_scores_gemma":[0.9851709,0.00017789766,0.0026272358,0.000062036306,0.000040853727,0.00003465442,0.0059925797,0.000038983824,0.00585485],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980825,0.00001541601,0.0000060561524,0.000045660145,0.00007615429,0.00004848238],"domain_scores_gemma":[0.99975127,0.000015542018,0.00009059742,0.000027353264,0.00004257496,0.000072649906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020675438,0.00030983146,0.00030585533,0.0012645026,0.00039522615,0.00038567532,0.0003360033,0.00025328022,0.0025532541],"category_scores_gemma":[0.00033275588,0.00024942032,0.00023594698,0.0006322089,0.00014370588,0.00015509724,0.000489919,0.00039540854,0.0005292459],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011797245,0.00046780868,0.54244906,0.00020504459,0.00047607237,0.001439429,0.00036421476,0.0042552585,0.36227682,0.0011722972,0.012602884,0.07311139],"study_design_scores_gemma":[0.000025893942,0.0001198514,0.98736143,0.000006110932,0.000027892434,0.00027144758,0.00003403415,0.0005774778,0.0033861673,0.000069112626,0.0081077395,0.00001288653],"about_ca_topic_score_codex":0.0062630223,"about_ca_topic_score_gemma":0.023097424,"teacher_disagreement_score":0.0062630223,"about_ca_system_score_codex":0.0007870158,"about_ca_system_score_gemma":0.00027545897,"threshold_uncertainty_score":0.012453139},"labels":[],"label_agreement":null},{"id":"W2167724286","doi":"10.1088/0004-637x/739/1/31","title":"THEORY OF SECULAR CHAOS AND MERCURY'S ORBIT","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Quantum chaos and dynamical systems","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Eccentricity (behavior); Orbital eccentricity; Venus; Nonlinear system; Planet; Orbit (dynamics); Celestial mechanics; Orbital elements","score_opus":0.012288862769963731,"score_gpt":0.20725376444391594,"score_spread":0.1949649016739522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167724286","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.514374,0.0017294692,0.4176984,0.0017079702,0.00014239045,0.00003359122,0.0001764288,0.00056013564,0.0635776],"genre_scores_gemma":[0.9873541,0.00039032323,0.008069903,0.00005687248,0.000044627795,0.000028271523,0.000031379972,0.00004020551,0.0039843167],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993074,0.000017828314,0.0000018965703,0.000009389371,0.000023534341,0.000016601438],"domain_scores_gemma":[0.9998,0.00008014104,0.000047381032,0.000018290899,0.000027315858,0.000026856997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001724066,0.00024074911,0.00025752178,0.0005573996,0.00040170056,0.00047158104,0.00045305936,0.00028763321,0.001983135],"category_scores_gemma":[0.0008659327,0.00010316329,0.00026958864,0.0003196939,0.0009532079,0.00077307766,0.00055509835,0.00032476947,0.00016382344],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027580907,0.000009196024,0.0018856983,0.00005950145,0.00003546433,0.00014867046,0.00023506039,0.38742292,0.002750413,0.5960335,0.001374402,0.010017652],"study_design_scores_gemma":[0.0000054089696,0.000014241307,0.0009199142,0.0000073054066,0.0000035373162,0.00004979568,0.000038250484,0.83034813,0.0003005704,0.16675298,0.0015514792,0.000008320883],"about_ca_topic_score_codex":0.0025175007,"about_ca_topic_score_gemma":0.0013224626,"teacher_disagreement_score":0.0025175007,"about_ca_system_score_codex":0.0006255577,"about_ca_system_score_gemma":0.00039517283,"threshold_uncertainty_score":0.0066342354},"labels":[],"label_agreement":null},{"id":"W2167738371","doi":"10.1086/526338","title":"Eight New Millisecond Pulsars in NGC 6440 and NGC 6441","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":197,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; University of British Columbia","funders":"","keywords":"Millisecond pulsar; Pulsar; Physics; Globular cluster; Astrophysics; Astronomy; Pulsar planet; Binary number; Binary pulsar; Galaxy","score_opus":0.014734525576332199,"score_gpt":0.28990041446856873,"score_spread":0.27516588889223653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167738371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99890316,0.00008479067,0.00015218035,0.000035127112,0.0000074610557,0.0000052158543,0.000059743146,0.000015788488,0.00073650165],"genre_scores_gemma":[0.99703133,0.00012589442,0.00095243135,0.00003938146,0.000015528069,0.000013214759,0.00043069076,0.000008562739,0.0013828995],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968874,0.000018621551,0.0000246039,0.000075726326,0.00009512758,0.000097329335],"domain_scores_gemma":[0.99915564,0.00012444086,0.00026179783,0.000128933,0.000080563426,0.00024862372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041078293,0.00033960617,0.00026665578,0.0015651382,0.0011396245,0.00084871054,0.00040375357,0.0007168869,0.0013425088],"category_scores_gemma":[0.0008836157,0.0003907845,0.00037597315,0.0015902951,0.00064167747,0.0005242764,0.001243923,0.00047910467,0.0002946002],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056886044,0.0001096913,0.8787859,0.00006580822,0.00010904473,0.0057079126,0.004016608,0.00091420714,0.06774785,0.0018497068,0.00074980344,0.039374758],"study_design_scores_gemma":[0.0000318579,0.00014152621,0.9890588,0.000011362968,0.000034301644,0.0019418338,0.00054106314,0.00042542085,0.0021875172,0.00068059156,0.0049193706,0.00002644838],"about_ca_topic_score_codex":0.0048622694,"about_ca_topic_score_gemma":0.00844895,"teacher_disagreement_score":0.0048622694,"about_ca_system_score_codex":0.0006208816,"about_ca_system_score_gemma":0.00034715215,"threshold_uncertainty_score":0.009667933},"labels":[],"label_agreement":null},{"id":"W2167755706","doi":"10.1088/0004-637x/738/2/139","title":"A SUNYAEV-ZEL'DOVICH-SELECTED SAMPLE OF THE MOST MASSIVE GALAXY CLUSTERS IN THE 2500 deg<sup>2</sup>SOUTH POLE TELESCOPE SURVEY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":270,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; South Pole Telescope; Redshift; Galaxy cluster; Sky; Cluster (spacecraft); Galaxy; Telescope; Sunyaev–Zel'dovich effect; Astronomy","score_opus":0.014415717077824474,"score_gpt":0.20782426598945397,"score_spread":0.1934085489116295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167755706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99498415,0.00011065139,0.00034120202,0.000029521321,0.0000023624768,0.000023434406,0.0032022654,0.000027096694,0.0012791958],"genre_scores_gemma":[0.9870803,0.00011479741,0.0010123863,0.000023034268,0.000010086303,0.000022782157,0.010447187,0.000015511032,0.0012738802],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998627,0.00001243869,0.000008903445,0.00004025572,0.00004180216,0.00003382667],"domain_scores_gemma":[0.99965954,0.000032595628,0.00009044563,0.00004091208,0.000044284796,0.00013213561],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021648317,0.00014597543,0.00020868979,0.0011654467,0.00029856415,0.00036802204,0.00021444584,0.00009976046,0.0019391997],"category_scores_gemma":[0.00043172328,0.0001289042,0.000106787214,0.0010501061,0.00015682408,0.00015041041,0.00042049843,0.00011381505,0.0005620878],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001319077,0.000030129871,0.96951675,0.000026712454,0.000029377705,0.00011327113,0.00027451236,0.0003872999,0.010542025,0.00023754075,0.002733359,0.01597716],"study_design_scores_gemma":[0.000003179977,0.000012591095,0.9981731,0.0000012289133,0.000004162962,0.000050106155,0.000048127604,0.00017064654,0.00027209465,0.000017124066,0.0012465816,0.0000011118265],"about_ca_topic_score_codex":0.009130812,"about_ca_topic_score_gemma":0.026533239,"teacher_disagreement_score":0.009130812,"about_ca_system_score_codex":0.00027231034,"about_ca_system_score_gemma":0.00027684963,"threshold_uncertainty_score":0.018155336},"labels":[],"label_agreement":null},{"id":"W2167952501","doi":"10.1088/0004-637x/690/2/1236","title":"COSMOS PHOTOMETRIC REDSHIFTS WITH 30-BANDS FOR 2-deg<sup>2</sup>","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1218,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Aspen Center for Physics; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; European Southern Observatory; Space Telescope Science Institute; National Science Foundation","keywords":"Redshift; Spectrograph; Telescope; Spectral energy distribution; Photometric redshift; Emission spectrum; Infrared; Very Large Telescope; Galaxy","score_opus":0.01924895988150692,"score_gpt":0.263096363897084,"score_spread":0.24384740401557709,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167952501","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2577948,0.0019776607,0.08670584,0.00067254016,0.0010236311,0.00058827223,0.47054607,0.024497172,0.15619408],"genre_scores_gemma":[0.4015833,0.0010009715,0.11364108,0.0004271496,0.00045907404,0.000613715,0.46239528,0.0038770798,0.016002236],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996203,0.000068155816,0.00004176103,0.000081154074,0.00013982251,0.00004886137],"domain_scores_gemma":[0.99919325,0.00010421859,0.00015362885,0.00029563328,0.00019364266,0.000059534494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007349209,0.0009701516,0.00033641388,0.0027389145,0.00022375789,0.00068305986,0.0006216031,0.00031756176,0.023596514],"category_scores_gemma":[0.0018621581,0.00040688133,0.0004998794,0.0036141104,0.00022286769,0.0006641074,0.00061683665,0.00051928754,0.012328845],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012899205,0.00020662692,0.2554769,0.00063457456,0.00032567413,0.00056797464,0.00043243487,0.019625183,0.017139519,0.02473035,0.47770032,0.20187047],"study_design_scores_gemma":[0.00015777718,0.00012729896,0.41582313,0.00010588679,0.00010850084,0.0010812532,0.00014000562,0.016994493,0.012741074,0.0069409753,0.5457067,0.00007290545],"about_ca_topic_score_codex":0.006556915,"about_ca_topic_score_gemma":0.0077763963,"teacher_disagreement_score":0.023596514,"about_ca_system_score_codex":0.00032268406,"about_ca_system_score_gemma":0.00025120546,"threshold_uncertainty_score":0.078938246},"labels":[],"label_agreement":null},{"id":"W2167965398","doi":"10.1088/0004-637x/745/2/130","title":"EARLY-TYPE GALAXIES AT<i>z</i>∼ 1.3. IV. SCALING RELATIONS IN DIFFERENT ENVIRONMENTS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Astrophysics; Physics; Photometry (optics); Scaling; Initial mass function; Stellar mass; Star formation; Astronomy; Stars; Mathematics; Geometry","score_opus":0.008934964243240338,"score_gpt":0.2055364315719609,"score_spread":0.19660146732872055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2167965398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949131,0.00030287405,0.0003242563,0.00003379653,0.0000027813196,0.0000062255513,0.0004853533,0.00003240283,0.0038993598],"genre_scores_gemma":[0.9989195,0.00006947804,0.00019182844,0.000010211573,0.000004844683,0.0000037091318,0.0003910293,0.0000047779913,0.00040461423],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998752,0.000009765411,0.000007348808,0.000041975698,0.000016112419,0.00004963221],"domain_scores_gemma":[0.9988673,0.00021417775,0.0004348549,0.00009595939,0.000109707114,0.00027811003],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024991448,0.00024149653,0.00014878924,0.0017791087,0.00022434832,0.0007688877,0.00019773291,0.00020155401,0.0028466445],"category_scores_gemma":[0.0010370995,0.00010728735,0.00029676067,0.00068284804,0.0003121149,0.00060165185,0.0005410415,0.0002959622,0.0005685683],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011770471,0.000018548117,0.9858431,0.000023961376,0.000025930125,0.000089497975,0.00036962164,0.00034576305,0.003876338,0.0011967476,0.00023446826,0.007858348],"study_design_scores_gemma":[0.0000013431272,0.000016673814,0.9986847,0.0000030414544,0.0000046567166,0.00006571493,0.00014364443,0.0002039505,0.00022504115,0.0003027803,0.00034646993,0.0000018794894],"about_ca_topic_score_codex":0.0027598932,"about_ca_topic_score_gemma":0.00346425,"teacher_disagreement_score":0.0028466445,"about_ca_system_score_codex":0.00030709154,"about_ca_system_score_gemma":0.000078126825,"threshold_uncertainty_score":0.009523034},"labels":[],"label_agreement":null},{"id":"W2168007549","doi":"10.1088/0004-637x/809/1/41","title":"TESTING THEORIES OF GRAVITATION USING 21-YEAR TIMING OF PULSAR BINARY J1713+0747","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Universities Space Research Association; National Science Foundation","keywords":"Pulsar; Physics; Binary pulsar; Gravitational wave; Astrophysics; Neutron star; Gravitational constant; White dwarf; Orbital period; Astronomy; Gravitational field; Millisecond pulsar","score_opus":0.05151594773484221,"score_gpt":0.3523699799736732,"score_spread":0.300854032238831,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168007549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99801046,0.00007665544,0.00037086502,0.00007960627,0.000023768023,0.0000071720556,0.00025314023,0.000008399317,0.00116997],"genre_scores_gemma":[0.9989222,0.000049975093,0.00022523597,0.000026397158,0.000015488296,0.000011347603,0.00059336337,0.000007094677,0.0001489774],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99925405,0.00023250193,0.00007648667,0.00016376036,0.00016334112,0.00010988228],"domain_scores_gemma":[0.9901276,0.004939866,0.0025042773,0.0007716252,0.00087878725,0.0007777927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023034578,0.00033288152,0.00047655246,0.0006614386,0.000818171,0.0011632368,0.0006599614,0.0006052877,0.0021513843],"category_scores_gemma":[0.011099259,0.00017764854,0.0006135225,0.00085147144,0.00075925444,0.00097274635,0.0013531329,0.0006177786,0.000277828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012248304,0.00025969066,0.9681684,0.00008263683,0.00038760682,0.0002553256,0.0005613321,0.0049616583,0.006044819,0.0067397836,0.0006319083,0.010681876],"study_design_scores_gemma":[0.00011406173,0.0010133113,0.97264355,0.000020707272,0.0002696811,0.00018201428,0.00087846123,0.01593854,0.002487916,0.0046126023,0.0018013245,0.000037799047],"about_ca_topic_score_codex":0.004835053,"about_ca_topic_score_gemma":0.0031151252,"teacher_disagreement_score":0.004835053,"about_ca_system_score_codex":0.00080303074,"about_ca_system_score_gemma":0.0011245908,"threshold_uncertainty_score":0.012181938},"labels":[],"label_agreement":null},{"id":"W2168017414","doi":"10.1088/0004-637x/760/2/136","title":"SEARCH FOR A CORRELATION BETWEEN VERY-HIGH-ENERGY GAMMA RAYS AND GIANT RADIO PULSES IN THE CRAB PULSAR","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Crab Pulsar; Astrophysics; Telescope; Gamma ray; Flux (metallurgy); Radio telescope; Crab Nebula; Astronomy","score_opus":0.019077856258750154,"score_gpt":0.3054233041162245,"score_spread":0.28634544785747434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168017414","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991929,0.00008238888,0.0003020753,0.000017339553,0.0000023897371,0.0000068776963,0.00010115707,0.000012165104,0.00028283108],"genre_scores_gemma":[0.9988361,0.000029382278,0.00071762514,0.000027218723,0.000009445778,0.000008818273,0.00025697364,0.0000074334394,0.00010707323],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996774,0.000057112953,0.000027834896,0.00010942741,0.00007511603,0.00005313926],"domain_scores_gemma":[0.9969969,0.00091400696,0.001213309,0.00021279893,0.0001744763,0.0004885191],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060486875,0.00020258575,0.00033937895,0.0011078095,0.0004205069,0.0008031237,0.00046619834,0.00043463567,0.0013761825],"category_scores_gemma":[0.0019129788,0.0002792996,0.0003141542,0.0009453267,0.000387531,0.00025352932,0.0006722148,0.000497409,0.00021282161],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001821287,0.00007347102,0.9762763,0.0000234609,0.00009495396,0.000329146,0.0001367148,0.00030218583,0.018806657,0.000059003592,0.000089700465,0.0036262476],"study_design_scores_gemma":[0.000008802371,0.00011759462,0.9978891,0.000004691791,0.000032173546,0.00027520926,0.00008981038,0.00055487273,0.00080324756,0.000022388258,0.00019672839,0.000005379919],"about_ca_topic_score_codex":0.0018509289,"about_ca_topic_score_gemma":0.0047545163,"teacher_disagreement_score":0.0018509289,"about_ca_system_score_codex":0.00022245283,"about_ca_system_score_gemma":0.00038456876,"threshold_uncertainty_score":0.004603803},"labels":[],"label_agreement":null},{"id":"W2168086026","doi":"10.1088/0004-637x/699/2/1038","title":"SUBARU WEAK LENSING MEASUREMENTS OF FOUR STRONG LENSING CLUSTERS: ARE LENSING CLUSTERS OVERCONCENTRATED?","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Weak gravitational lensing; Astrophysics; Physics; Redshift; Strong gravitational lensing; Dark matter; Cluster (spacecraft); Gravitational lensing formalism; Lens (geology); Galaxy; Optics","score_opus":0.026807546820275138,"score_gpt":0.23444494608353753,"score_spread":0.20763739926326238,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168086026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99861133,0.00003602688,0.00070311845,0.000009049856,5.9670174e-7,0.0000024951294,0.0001627852,0.00001874212,0.0004558652],"genre_scores_gemma":[0.99884474,0.000018995064,0.00073462323,0.000003885078,0.0000018906301,0.0000023809714,0.00030761005,0.0000051333036,0.00008075385],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983764,0.000018398498,0.000010035951,0.000048085818,0.000051150924,0.000034681616],"domain_scores_gemma":[0.9991923,0.00012360187,0.0003293558,0.00010853681,0.0001067211,0.0001394358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024576727,0.00032063495,0.00023640411,0.0010979495,0.0002582136,0.0004496998,0.0003516464,0.00019340025,0.00057805236],"category_scores_gemma":[0.0011710146,0.0002416437,0.00027065768,0.00056543597,0.00029598645,0.00028758385,0.000763548,0.00015656231,0.0002312715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001692842,0.000020804218,0.94286215,0.00003240711,0.00008687145,0.00010681091,0.0001976773,0.006088411,0.039574865,0.00067167956,0.0001547343,0.010034206],"study_design_scores_gemma":[0.00000474019,0.000030539177,0.9763689,0.00000264565,0.000024712379,0.00006457307,0.00006951835,0.01596462,0.006989501,0.00018812175,0.00028251734,0.000009688033],"about_ca_topic_score_codex":0.009169558,"about_ca_topic_score_gemma":0.01322189,"teacher_disagreement_score":0.009169558,"about_ca_system_score_codex":0.0004948107,"about_ca_system_score_gemma":0.0001878241,"threshold_uncertainty_score":0.018232346},"labels":[],"label_agreement":null},{"id":"W2168179538","doi":"10.1088/0004-637x/761/2/171","title":"FILAMENTARY STAR FORMATION: OBSERVING THE EVOLUTION TOWARD FLATTENED ENVELOPES","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Millimeter; Submillimeter Array; Astrophysics; Star formation; Envelope (radar); Molecular cloud; Wavelength; Scale (ratio); Astronomy; Circumstellar envelope; Stars; Optics; Computer science","score_opus":0.021514708196774902,"score_gpt":0.23845644152087586,"score_spread":0.21694173332410097,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168179538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99583,0.00009369723,0.003067237,0.00002408208,0.000003381721,0.000006931063,0.00024959372,0.000084642175,0.00064048177],"genre_scores_gemma":[0.99654573,0.000039103146,0.002885051,0.00001036233,0.000004203062,0.0000034234813,0.00043954974,0.000008678221,0.00006408199],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994874,0.000008083566,0.0000020408152,0.000018194132,0.000009475438,0.000013504637],"domain_scores_gemma":[0.999897,0.000018841925,0.000028380922,0.000018459648,0.000010622454,0.00002674078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012570436,0.0002096159,0.00015018097,0.00033675658,0.00014301541,0.00029866322,0.00029169774,0.00027183513,0.00038332577],"category_scores_gemma":[0.0002700939,0.00013713649,0.00030770904,0.00032328203,0.00012282733,0.00024363348,0.00024225134,0.00019931117,0.00006186905],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005923555,0.0003117066,0.60108393,0.00012626918,0.00042081336,0.0011518005,0.0004752256,0.15675744,0.20193718,0.0017526987,0.0010872567,0.034303285],"study_design_scores_gemma":[0.00004638547,0.00017302652,0.6762848,0.00001440665,0.00008177482,0.00039166733,0.00016166235,0.3039998,0.01611457,0.0009349155,0.0017651449,0.000031924712],"about_ca_topic_score_codex":0.003191503,"about_ca_topic_score_gemma":0.003158492,"teacher_disagreement_score":0.003191503,"about_ca_system_score_codex":0.00019989393,"about_ca_system_score_gemma":0.00007525302,"threshold_uncertainty_score":0.006345868},"labels":[],"label_agreement":null},{"id":"W2168233992","doi":"10.1088/0004-637x/698/1/594","title":"AN ENERGETIC AGN OUTBURST POWERED BY A RAPIDLY SPINNING SUPERMASSIVE BLACK HOLE OR AN ACCRETING ULTRAMASSIVE BLACK HOLE","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Supermassive black hole; Solar mass; Intermediate-mass black hole; Stellar black hole; Black hole (networking); Accretion (finance); Spin-flip; Cooling flow","score_opus":0.01290549932188809,"score_gpt":0.25818957238650464,"score_spread":0.24528407306461655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168233992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99431866,0.0002014756,0.0009005366,0.00009776705,0.000023491026,0.000008136419,0.000079059566,0.000071557864,0.0042993533],"genre_scores_gemma":[0.99880946,0.00007352112,0.000288213,0.000058606867,0.000021675341,0.0000029457092,0.00006437417,0.000002882028,0.000678328],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999665,0.0000020282046,0.0000021856379,0.000009817756,0.0000066513817,0.000012859985],"domain_scores_gemma":[0.99985874,0.00001894804,0.00006459908,0.000014905799,0.0000065797926,0.00003625218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009549219,0.00019052466,0.00014193809,0.00023119323,0.0002786729,0.00040896467,0.00019869319,0.00029155763,0.0018551128],"category_scores_gemma":[0.00022903671,0.0000863569,0.00021863967,0.00012295764,0.000228873,0.0002021466,0.0003387515,0.00017457762,0.00020941574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066496414,0.00014688235,0.65567124,0.00020052459,0.00014507893,0.009552431,0.00081211026,0.0042786086,0.2850302,0.011055102,0.0022742564,0.03016861],"study_design_scores_gemma":[0.00005376772,0.0002801941,0.96150357,0.000035623834,0.000105117586,0.0063449,0.00039395495,0.0072016097,0.014728352,0.0036490445,0.005678697,0.000025184518],"about_ca_topic_score_codex":0.0012886813,"about_ca_topic_score_gemma":0.0023749357,"teacher_disagreement_score":0.0018551128,"about_ca_system_score_codex":0.00024037296,"about_ca_system_score_gemma":0.00009004387,"threshold_uncertainty_score":0.0062059164},"labels":[],"label_agreement":null},{"id":"W2168283625","doi":"10.1086/503893","title":"On the Viability of Bianchi Type VII<sub><i>h</i></sub>Models with Dark Energy","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"","keywords":"CMB cold spot; Dark energy; Physics; Cosmic microwave background; Degeneracy (biology); Anisotropy; Astrophysics; Cosmology; Lambda-CDM model; Type (biology); Universe; Mathematical physics; Theoretical physics; De Sitter universe; Quantum mechanics","score_opus":0.005416357108649241,"score_gpt":0.19732754310566047,"score_spread":0.19191118599701124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168283625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.83365726,0.001519041,0.07358326,0.009855348,0.00028244138,0.000065520486,0.0005775475,0.00029473842,0.08016486],"genre_scores_gemma":[0.9905481,0.00045982676,0.0049646995,0.00028328525,0.00028767996,0.00002549927,0.0002774814,0.00006441224,0.0030890661],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99900204,0.00046741456,0.00003754784,0.00012749457,0.0001739257,0.00019172048],"domain_scores_gemma":[0.99431956,0.0021970144,0.0011182094,0.0013615864,0.0003921075,0.00061152445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004026023,0.0010021047,0.00094109226,0.0010273771,0.0017886006,0.0039284937,0.0020195327,0.0016357726,0.005439745],"category_scores_gemma":[0.009297464,0.0003601757,0.001031365,0.000872048,0.0021753977,0.0033740816,0.0025998843,0.00152009,0.0010969024],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004561653,0.0001437568,0.026071876,0.000114913666,0.00020553207,0.0006694378,0.0004943257,0.037111018,0.0015789357,0.90982103,0.004932737,0.018400397],"study_design_scores_gemma":[0.00011152702,0.00012207123,0.008480238,0.00006139508,0.00009631346,0.00041615052,0.0003136279,0.2963731,0.00060517504,0.68856955,0.004783258,0.00006759703],"about_ca_topic_score_codex":0.004876725,"about_ca_topic_score_gemma":0.004983464,"teacher_disagreement_score":0.005439745,"about_ca_system_score_codex":0.0010064226,"about_ca_system_score_gemma":0.0009577414,"threshold_uncertainty_score":0.021291912},"labels":[],"label_agreement":null},{"id":"W2168375973","doi":"10.1086/508567","title":"AEGIS: Infrared Spectroscopy of an Infrared-luminous Lyman Break Galaxy at <i>z</i>  = 3.01","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cosmic infrared background; Infrared; Galaxy; Spectroscopy; Infrared astronomy; Infrared spectroscopy; Ultraviolet astronomy; Astronomical spectroscopy","score_opus":0.00467942704652356,"score_gpt":0.20309182853060936,"score_spread":0.19841240148408582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168375973","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.934627,0.0013696112,0.0029525782,0.0009923944,0.00021483639,0.000096129894,0.01267279,0.001713097,0.045361612],"genre_scores_gemma":[0.9762763,0.0006618398,0.008198755,0.00037766315,0.00009869159,0.000034677756,0.0075473916,0.0002836351,0.0065210387],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999255,0.0000043964583,0.000004029011,0.00001809632,0.000025607767,0.00002233057],"domain_scores_gemma":[0.99985015,0.000010802901,0.00003688204,0.00002695282,0.000016999285,0.00005821393],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031578503,0.00032612536,0.0002625961,0.00092049246,0.0005391576,0.0005410247,0.0005370255,0.00043437848,0.005398698],"category_scores_gemma":[0.00015267047,0.00021280738,0.00022115961,0.00054570637,0.00020048831,0.00044649257,0.0005454453,0.00059032347,0.0011683383],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015923654,0.00044624874,0.26573554,0.00025486498,0.0003990871,0.0037960128,0.0007545199,0.0012864263,0.59683347,0.0032349343,0.061788294,0.063878246],"study_design_scores_gemma":[0.00010831508,0.00016914099,0.9505549,0.00003350338,0.00009926449,0.0013883376,0.00030948632,0.00207058,0.022739395,0.00076037523,0.021733524,0.00003328459],"about_ca_topic_score_codex":0.006263711,"about_ca_topic_score_gemma":0.014921298,"teacher_disagreement_score":0.006263711,"about_ca_system_score_codex":0.00042012386,"about_ca_system_score_gemma":0.00016827574,"threshold_uncertainty_score":0.018060446},"labels":[],"label_agreement":null},{"id":"W2168609373","doi":"10.1088/0004-637x/767/1/88","title":"ALMA REDSHIFTS OF MILLIMETER-SELECTED GALAXIES FROM THE SPT SURVEY: THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":304,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Redshift; Galaxy; Luminous infrared galaxy; Astronomy; Redshift survey; Millimeter; Radio galaxy; Red shift","score_opus":0.010614420432282702,"score_gpt":0.2087844275054358,"score_spread":0.1981700070731531,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168609373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99591523,0.00007659876,0.0004923653,0.000032367458,0.000004209341,0.000009453557,0.0022247536,0.0000912701,0.001153886],"genre_scores_gemma":[0.9952036,0.000058040954,0.00056396145,0.0000199132,0.000013654866,0.000013808409,0.003694901,0.000015866333,0.0004163137],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999699,0.00004492672,0.000021032745,0.0000884004,0.000087308195,0.00005933365],"domain_scores_gemma":[0.9986733,0.00016504293,0.0004909813,0.00017950093,0.00021689809,0.0002742942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055110594,0.00023154906,0.00023889107,0.002764146,0.0002671082,0.000584988,0.00030029236,0.0002573026,0.0020431322],"category_scores_gemma":[0.0014710859,0.00013559034,0.0002412871,0.0016552559,0.00021678183,0.00031143543,0.0006618775,0.00031321426,0.0007186627],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006482888,0.00001834285,0.98853475,0.000013827356,0.000040608393,0.00005790676,0.00024148928,0.00014475123,0.0038990492,0.00013244073,0.0005219577,0.006330094],"study_design_scores_gemma":[0.0000029280209,0.000013170874,0.99901485,0.0000011189852,0.000005880663,0.00004709224,0.00004327749,0.00021068194,0.00025773735,0.000019739344,0.00038207226,0.0000015176616],"about_ca_topic_score_codex":0.0055137384,"about_ca_topic_score_gemma":0.0056967977,"teacher_disagreement_score":0.0055137384,"about_ca_system_score_codex":0.0002850743,"about_ca_system_score_gemma":0.000116808464,"threshold_uncertainty_score":0.010963261},"labels":[],"label_agreement":null},{"id":"W2168670288","doi":"10.1088/0004-637x/747/1/10","title":"X-RAY AND MULTIWAVELENGTH INSIGHTS INTO THE NATURE OF WEAK EMISSION-LINE QUASARS AT LOW REDSHIFT","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Ludwig-Maximilians-Universität München; Max-Planck-Gesellschaft; Alfred P. Sloan Foundation; Georg-August-Universität Göttingen; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Quasar; Astrophysics; Physics; OVV quasar; Redshift; Emission spectrum; Astronomy; Sky; Brightness; Spectral line; Line (geometry); Galaxy","score_opus":0.005915524710657145,"score_gpt":0.22206147814447852,"score_spread":0.21614595343382137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2168670288","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975794,0.00078398065,0.00029541823,0.0000361354,0.0000028788793,0.0000021432695,0.00025018555,0.000015072716,0.0010348214],"genre_scores_gemma":[0.99790466,0.00035027252,0.00046913588,0.000049073886,0.00002157311,0.0000024545766,0.00051551533,0.0000072662438,0.00068011857],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999403,0.000005427677,0.0000057763764,0.000015000338,0.000015048481,0.00001858367],"domain_scores_gemma":[0.9996094,0.000050615236,0.00019210139,0.00002727489,0.000036927355,0.0000836852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023611107,0.00029032715,0.00018891018,0.0014322746,0.0001906844,0.0005444174,0.0001779337,0.00017173326,0.0019951805],"category_scores_gemma":[0.00027015753,0.00011410714,0.00018790382,0.0006221949,0.00022067073,0.00033738272,0.00040980297,0.00026319717,0.00037672298],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019908798,0.000052524498,0.87347424,0.000091020986,0.000057236863,0.0007822401,0.00037038288,0.00025139397,0.107243754,0.00041156792,0.00033998213,0.016726658],"study_design_scores_gemma":[0.0000015373286,0.00003815275,0.9978617,0.000003238802,0.000009315326,0.00034182004,0.000076517885,0.000073216295,0.0010638415,0.00006924731,0.00045892762,0.00000242461],"about_ca_topic_score_codex":0.0009910837,"about_ca_topic_score_gemma":0.0017668566,"teacher_disagreement_score":0.0019951805,"about_ca_system_score_codex":0.00012753777,"about_ca_system_score_gemma":0.000041766747,"threshold_uncertainty_score":0.006674528},"labels":[],"label_agreement":null},{"id":"W2169039585","doi":"10.1086/591513","title":"The Resolved Properties of Extragalactic Giant Molecular Clouds","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":526,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Astrophysics; Physics; Virial theorem; Galaxy; Luminosity; Star formation; Molecular cloud; Metallicity; Local Group; Small Magellanic Cloud; Virial mass; Spiral galaxy; Line (geometry); Astronomy; Milky Way; Stars","score_opus":0.016849209465734177,"score_gpt":0.2208307907747788,"score_spread":0.20398158130904462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169039585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99806494,0.00040378008,0.00016372203,0.000009458372,0.0000020098569,0.0000017101527,0.00054346316,0.000010780312,0.0008001902],"genre_scores_gemma":[0.9987356,0.00011092579,0.00018800961,0.000008626654,0.0000037511754,9.5298714e-7,0.00077529316,0.0000026263858,0.00017420763],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988914,0.0000072526686,0.0000051986885,0.000050094455,0.000027706476,0.000020574415],"domain_scores_gemma":[0.99958545,0.000057758723,0.00015088235,0.0000545461,0.00006484581,0.00008660645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016144864,0.0001816996,0.00018184552,0.0009785569,0.00017148077,0.0005524134,0.00024631573,0.00019501163,0.00082895433],"category_scores_gemma":[0.00037007846,0.00011656734,0.00014461906,0.0007183757,0.00017607198,0.00043232518,0.0005220053,0.00020680802,0.00019743804],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014180894,0.00003905347,0.8991277,0.00008985463,0.00021092827,0.00011759423,0.00020897607,0.0012848253,0.086435735,0.0003956118,0.0003610817,0.0115867425],"study_design_scores_gemma":[0.0000023512737,0.000024150031,0.9940041,0.0000052153646,0.000024309404,0.00008934299,0.000077302146,0.0005925797,0.0047006244,0.00005614328,0.00041986164,0.0000040474347],"about_ca_topic_score_codex":0.0020192973,"about_ca_topic_score_gemma":0.004202649,"teacher_disagreement_score":0.0020192973,"about_ca_system_score_codex":0.0002152078,"about_ca_system_score_gemma":0.000058842506,"threshold_uncertainty_score":0.004015088},"labels":[],"label_agreement":null},{"id":"W2169042857","doi":"10.1086/381751","title":"The Extragalactic Origin of the Arcturus Group","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Stars; Galaxy; Galactic plane; Population; Galactic Center; Accretion (finance); Stellar population; K-type main-sequence star","score_opus":0.01150369775617209,"score_gpt":0.2654248058960515,"score_spread":0.2539211081398794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169042857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99592245,0.00038467327,0.00018853217,0.00006589679,0.00000767469,0.0000031092,0.00008097547,0.000018811576,0.0033278414],"genre_scores_gemma":[0.9987721,0.00022250689,0.00042427308,0.000014916945,0.000009293747,0.0000020501247,0.00017554086,0.0000073298365,0.00037193872],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986076,0.000016469034,0.000006850233,0.000039141512,0.000036023102,0.00004079485],"domain_scores_gemma":[0.99953735,0.000028343995,0.00017098931,0.00007227849,0.00007123057,0.00011981482],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010677347,0.00012379634,0.00020418872,0.0010502296,0.00039488325,0.0006107087,0.000238164,0.00016087636,0.0019937379],"category_scores_gemma":[0.0007992823,0.00006995151,0.00012314315,0.000949317,0.0003082546,0.0003288848,0.00082112884,0.00024821234,0.00042894526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012539387,0.000021977368,0.9462069,0.000051203115,0.000048543967,0.00070120214,0.0011796078,0.00024139088,0.008144217,0.0019041464,0.00041502435,0.04096034],"study_design_scores_gemma":[0.0000043243085,0.00002920522,0.99086297,0.000018409493,0.000033378103,0.0010775945,0.00044135234,0.00021511252,0.00048386704,0.0005845012,0.006244423,0.000004867759],"about_ca_topic_score_codex":0.00432636,"about_ca_topic_score_gemma":0.0035952146,"teacher_disagreement_score":0.00432636,"about_ca_system_score_codex":0.00031242036,"about_ca_system_score_gemma":0.00024270536,"threshold_uncertainty_score":0.008602381},"labels":[],"label_agreement":null},{"id":"W2169155351","doi":"10.1086/500110","title":"The Gas Phase Spectrum of Cyclic C<sub>18</sub>and the Diffuse Interstellar Bands","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Ion; Absorption (acoustics); Phase (matter); Interstellar medium; Absorption spectroscopy; Molecule; Wavelength; Molecular cloud; Carbon monoxide; Atomic physics; Molecular physics; Stars; Optics; Galaxy; Chemistry","score_opus":0.0034326152923762087,"score_gpt":0.21777824589388123,"score_spread":0.21434563060150502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169155351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9811112,0.0005096142,0.00041946713,0.00023482025,0.00006380863,0.000011955126,0.0010228205,0.00009334368,0.016532898],"genre_scores_gemma":[0.9906624,0.0002459838,0.00038458858,0.00010407359,0.000046177134,0.000008023679,0.0010425881,0.000031394236,0.0074747666],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999721,0.0000012129351,4.5888748e-7,0.0000079353595,0.000008691258,0.000009620392],"domain_scores_gemma":[0.99984443,0.000023893432,0.000030489397,0.000008929413,0.00003492168,0.000057286376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004698562,0.00020536414,0.00009575836,0.00044546273,0.0003527692,0.00022202735,0.00020774062,0.00026539672,0.018072128],"category_scores_gemma":[0.00014935555,0.00008299047,0.0000781056,0.000373778,0.00022901228,0.00022613964,0.00018770558,0.00026372063,0.0012901826],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013362769,0.00012584223,0.064852454,0.00015491899,0.000040099036,0.0011183849,0.00018679883,0.00027891854,0.87779194,0.001951778,0.0064496757,0.045713004],"study_design_scores_gemma":[0.0000954313,0.00041008947,0.8418091,0.000025451707,0.000046246336,0.001202534,0.0003254749,0.0014604945,0.13125288,0.0010349569,0.02231375,0.0000236809],"about_ca_topic_score_codex":0.0013476035,"about_ca_topic_score_gemma":0.0020335577,"teacher_disagreement_score":0.018072128,"about_ca_system_score_codex":0.00014742347,"about_ca_system_score_gemma":0.00009628201,"threshold_uncertainty_score":0.06045729},"labels":[],"label_agreement":null},{"id":"W2169248600","doi":"10.1086/505558","title":"Cosmological Parameters from the 2003 Flight of BOOMERANG","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":180,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Polarization (electrochemistry); Spectral density; Redshift; Spectral line; Cosmic background radiation; Equation of state; Cosmology","score_opus":0.007971907990981025,"score_gpt":0.19829931361284878,"score_spread":0.19032740562186776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169248600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7899803,0.00083487673,0.0017038218,0.00084545836,0.00009461517,0.00006606085,0.14978379,0.00045517005,0.05623589],"genre_scores_gemma":[0.85323143,0.00065384485,0.0050674155,0.00023925971,0.000050977585,0.00005718526,0.13232593,0.00029892864,0.008074981],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992645,0.000008095143,0.0000024717958,0.000017162689,0.000023067076,0.000022658747],"domain_scores_gemma":[0.9997031,0.000026255388,0.00008294787,0.00004138817,0.000072636634,0.00007358185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018006301,0.000451302,0.00020776382,0.0016316483,0.00068579713,0.00045185644,0.00022304284,0.00020428708,0.0049811588],"category_scores_gemma":[0.0006032999,0.0001425971,0.00022729633,0.0021905776,0.00017954166,0.00024161466,0.0003661989,0.0005226785,0.0013730766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007895876,0.00021571195,0.6366375,0.00038664456,0.00034374255,0.0008026194,0.0025091271,0.014196792,0.010675396,0.011041292,0.21216688,0.11023471],"study_design_scores_gemma":[0.000020470306,0.000031681033,0.8766874,0.000029308942,0.00004356279,0.00040645222,0.0002796528,0.001772651,0.0014367814,0.0011551956,0.118079424,0.00005737284],"about_ca_topic_score_codex":0.14296436,"about_ca_topic_score_gemma":0.26005477,"teacher_disagreement_score":0.14296436,"about_ca_system_score_codex":0.0008122753,"about_ca_system_score_gemma":0.0004338432,"threshold_uncertainty_score":0.28426445},"labels":[],"label_agreement":null},{"id":"W2169318301","doi":"10.1088/0004-637x/794/1/12","title":"SPT-CL J2040–4451: AN SZ-SELECTED GALAXY CLUSTER AT<i>z</i>= 1.478 WITH SIGNIFICANT ONGOING STAR FORMATION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"Jet Propulsion Laboratory; Office of Science; McGill University; University of Chicago; Deutsche Forschungsgemeinschaft; Massachusetts Institute of Technology; California Institute of Technology; U.S. Department of Energy; Gordon and Betty Moore Foundation; Kavli Institute for Cosmological Physics, University of Chicago; Canada Research Chairs; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy cluster; Redshift; Galaxy; Cluster (spacecraft); Astronomy; Star formation; South Pole Telescope; Velocity dispersion","score_opus":0.005879506672908425,"score_gpt":0.19157798707422166,"score_spread":0.18569848040131323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169318301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99789655,0.000017170943,0.00008003508,0.00002648513,0.0000043503182,0.000013729211,0.0005882779,0.00004669082,0.0013266065],"genre_scores_gemma":[0.99493164,0.000022105864,0.0003941475,0.000038705428,0.000016277505,0.000011897423,0.0038027647,0.000013554733,0.00076888024],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982363,0.000005633092,0.000006636885,0.000043719727,0.000053051528,0.000067328976],"domain_scores_gemma":[0.9995652,0.000013323021,0.00009419139,0.000019066609,0.00003310095,0.00027516534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001362304,0.00032923208,0.00028339148,0.0012620294,0.0009585018,0.00051992026,0.0005432705,0.00031500746,0.003245769],"category_scores_gemma":[0.00023809793,0.0001608193,0.00022313792,0.0010083632,0.0004061878,0.00028111032,0.0010089498,0.00035443585,0.00083329703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043299,0.0002866032,0.9612137,0.00004935358,0.00007426938,0.0026451857,0.00049933075,0.00033553987,0.018857177,0.00033163192,0.0041143955,0.011159756],"study_design_scores_gemma":[0.00001852997,0.00012146129,0.99590105,0.000003069077,0.000014198049,0.000896527,0.00022102338,0.00064174057,0.00071178307,0.000042103715,0.0014216151,0.000006889163],"about_ca_topic_score_codex":0.011966916,"about_ca_topic_score_gemma":0.021374762,"teacher_disagreement_score":0.011966916,"about_ca_system_score_codex":0.0004617762,"about_ca_system_score_gemma":0.0003390368,"threshold_uncertainty_score":0.023794532},"labels":[],"label_agreement":null},{"id":"W2169330880","doi":"10.1086/503290","title":"Interferometric 890 μm Images of High-Redshift Submillimeter Galaxies","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Submillimeter Array; Physics; Astrophysics; Galaxy; Redshift; Astronomy; Luminosity; Interferometry; Star formation","score_opus":0.0057662171740887995,"score_gpt":0.1984613207197263,"score_spread":0.1926951035456375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169330880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98359114,0.00036290608,0.002274858,0.000080919555,0.000019626486,0.000020079524,0.0043881666,0.0004593626,0.00880299],"genre_scores_gemma":[0.9804113,0.0002989653,0.007134721,0.000089764806,0.0000509555,0.000020244548,0.010255937,0.000034574,0.0017036147],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999293,0.0000037669545,0.0000032668027,0.0000141551745,0.000026052216,0.000023480256],"domain_scores_gemma":[0.99985445,0.0000133119,0.000049502512,0.00002143378,0.000017816808,0.000043522632],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012441527,0.00016877615,0.00017441506,0.0011570107,0.00017264858,0.00022095285,0.00022892299,0.00017747164,0.002948075],"category_scores_gemma":[0.0001652341,0.0001497113,0.00020839511,0.0010785506,0.00007485394,0.00013579502,0.00019664221,0.00019535534,0.0008580429],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009438269,0.00049911585,0.28046843,0.0002943259,0.0003303345,0.0011662652,0.0005119852,0.0029486353,0.57363915,0.001993258,0.013248476,0.1239562],"study_design_scores_gemma":[0.000017412152,0.000060514245,0.98450536,0.000004966014,0.00003385321,0.0005189979,0.00003749447,0.0010969068,0.007435327,0.00014699093,0.006134666,0.0000076244696],"about_ca_topic_score_codex":0.0017157904,"about_ca_topic_score_gemma":0.0038059964,"teacher_disagreement_score":0.002948075,"about_ca_system_score_codex":0.00022218765,"about_ca_system_score_gemma":0.00007966132,"threshold_uncertainty_score":0.009862304},"labels":[],"label_agreement":null},{"id":"W2169351262","doi":"10.1086/308465","title":"Gas‐Phase Electronic Spectra of Carbon‐Chain Radicals Compared with Diffuse Interstellar Band Observations","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric chemistry and aerosols","field":"Earth and Planetary Sciences","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Dominion Astrophysical Observatory; University of British Columbia","funders":"","keywords":"Physics; Spectral line; Astrophysics; Carbon chain; Absorption spectroscopy; Absorption (acoustics); Interstellar medium; Carbon fibers; Interstellar cloud; Phase (matter); Atomic physics; Molecular cloud; Astronomy; Stars; Optics; Chemistry; Materials science; Composite number","score_opus":0.011230578537415653,"score_gpt":0.20459226092657581,"score_spread":0.19336168238916016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169351262","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99712867,0.00034745896,0.000390613,0.0000118673015,0.000005216419,0.0000034703737,0.00014014814,0.0000234065,0.0019491762],"genre_scores_gemma":[0.99879897,0.0001370581,0.00031320986,0.000011927767,0.0000067186984,0.000003027309,0.0002699397,0.0000057241623,0.00045338913],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999541,0.0000036130634,0.0000010298388,0.000020838095,0.000010306618,0.000010139253],"domain_scores_gemma":[0.9999167,0.000017308812,0.000018024957,0.0000073367814,0.000020077461,0.000020674803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059192625,0.00015161248,0.00007215512,0.0004511332,0.0001794987,0.00016268676,0.00012247587,0.00017231029,0.0020033515],"category_scores_gemma":[0.00013692533,0.000059527396,0.000055088014,0.00024148662,0.0001378577,0.0002068238,0.00019052647,0.00018758069,0.00022275763],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034239836,0.00003809371,0.03455445,0.000069711015,0.000021638694,0.00009248068,0.00012039585,0.00013060648,0.95527154,0.00018587333,0.000120688535,0.009052081],"study_design_scores_gemma":[0.000047678415,0.00058909523,0.6537883,0.000021183736,0.00005969466,0.00065491116,0.00034961256,0.0013162335,0.33859152,0.0002884654,0.0042774724,0.000015791768],"about_ca_topic_score_codex":0.00060790527,"about_ca_topic_score_gemma":0.001015034,"teacher_disagreement_score":0.0020033515,"about_ca_system_score_codex":0.00012758837,"about_ca_system_score_gemma":0.0000415994,"threshold_uncertainty_score":0.006701827},"labels":[],"label_agreement":null},{"id":"W2169456213","doi":"10.1088/0004-637x/717/2/1157","title":"THE BOLOCAM GALACTIC PLANE SURVEY. III. CHARACTERIZING PHYSICAL PROPERTIES OF MASSIVE STAR-FORMING REGIONS IN THE GEMINI OB1 MOLECULAR CLOUD","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"","keywords":"Virial theorem; Molecular cloud; Millimeter; Galactic plane; Line (geometry); RADIUS; Mean kinetic temperature; Isothermal process; Kinetic energy","score_opus":0.015871698222214955,"score_gpt":0.23771595471703358,"score_spread":0.22184425649481862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169456213","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9599362,0.0023146684,0.000507733,0.0002541629,0.000016724482,0.000048076672,0.031072421,0.00012080539,0.0057291845],"genre_scores_gemma":[0.93983984,0.0016473862,0.0014759218,0.00014325952,0.000052402524,0.000047810245,0.05473014,0.000028119597,0.0020352157],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.000017435721,0.0000067719493,0.000029310853,0.000032005646,0.000036517347],"domain_scores_gemma":[0.99962115,0.000018172188,0.0001872199,0.000029451763,0.00005837074,0.00008554199],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025181408,0.00028852583,0.00015545006,0.0019144772,0.00019554078,0.00051312067,0.00024364739,0.0001691804,0.0013315787],"category_scores_gemma":[0.0004082184,0.00012030614,0.00014691071,0.0013709259,0.00009997893,0.00018101688,0.000440559,0.00018036614,0.00066621165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013748198,0.000016870423,0.97383976,0.00005460125,0.00008421106,0.00007847949,0.00017784773,0.0001304494,0.0052969065,0.00015938185,0.004799723,0.015224199],"study_design_scores_gemma":[0.000005130329,0.0000061142437,0.99670297,0.0000065203826,0.000008092444,0.000046413395,0.00004094421,0.00005228237,0.00019922509,0.000011479743,0.0029198427,0.0000010536871],"about_ca_topic_score_codex":0.041727323,"about_ca_topic_score_gemma":0.054054745,"teacher_disagreement_score":0.041727323,"about_ca_system_score_codex":0.0006272057,"about_ca_system_score_gemma":0.00021861255,"threshold_uncertainty_score":0.08296889},"labels":[],"label_agreement":null},{"id":"W2169803721","doi":"10.1086/588541","title":"The Balloon‐borne Large Aperture Submillimeter Telescope: BLAST","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":148,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of British Columbia; University of Toronto","funders":"","keywords":"Telescope; Milky Way; Galaxy; Aperture (computer memory); Galactic astronomy; Raster graphics; Detector; Sky; Spectral resolution","score_opus":0.011251794074413577,"score_gpt":0.22402031303106615,"score_spread":0.21276851895665258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2169803721","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.82830274,0.0022289073,0.07114882,0.0011208254,0.000440985,0.0007283945,0.020398052,0.011153452,0.06447782],"genre_scores_gemma":[0.8867679,0.00047693925,0.08608739,0.00039829328,0.00018968765,0.00025589098,0.017647631,0.0005340603,0.007642266],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99926776,0.00008596621,0.000018986062,0.0001832028,0.00029247065,0.0001517192],"domain_scores_gemma":[0.99918395,0.00009427587,0.0001242249,0.00018235325,0.00021385169,0.00020137806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014690002,0.00041294825,0.00060261914,0.0006735107,0.0006366625,0.0006221807,0.000625344,0.00058627955,0.0027411985],"category_scores_gemma":[0.00108484,0.00033097243,0.00025808343,0.0012013626,0.00035111693,0.0007867331,0.0009438624,0.0006413125,0.001559207],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0061096014,0.00041455973,0.16759326,0.00054634106,0.0003190924,0.00072541717,0.0014693404,0.0069517656,0.45391494,0.008835368,0.08099965,0.2721207],"study_design_scores_gemma":[0.00096861663,0.0027516799,0.5060289,0.00012606008,0.0002949282,0.0032754946,0.00042933106,0.05166655,0.14332634,0.00419306,0.28668684,0.0002522243],"about_ca_topic_score_codex":0.0020874925,"about_ca_topic_score_gemma":0.0026188341,"teacher_disagreement_score":0.0027411985,"about_ca_system_score_codex":0.00066724257,"about_ca_system_score_gemma":0.00060180266,"threshold_uncertainty_score":0.009170175},"labels":[],"label_agreement":null},{"id":"W2170084055","doi":"10.1088/0004-637x/787/2/129","title":"INVESTIGATING CXOU J163802.6–471358: A NEW PULSAR WIND NEBULA IN THE NORMA REGION?","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Galactic plane; Point source; Source counts; Pulsar wind nebula; Astrometry; Nebula; Spiral galaxy; Power law","score_opus":0.019544768469028796,"score_gpt":0.23827002531318256,"score_spread":0.21872525684415375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2170084055","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808794,0.00028963925,0.0003467186,0.000043144042,0.000006565747,0.000009571582,0.00013177635,0.00001305645,0.0010714937],"genre_scores_gemma":[0.9965145,0.0002580808,0.0016245442,0.0000786015,0.000032270207,0.0000092749515,0.00083377026,0.0000136318,0.0006352888],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999285,0.0000044764297,0.0000037935174,0.000022339136,0.00001846308,0.00002237534],"domain_scores_gemma":[0.99973303,0.00003010064,0.0001067424,0.000021150552,0.00002530395,0.00008366849],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021193,0.00026586704,0.00036357224,0.0007950383,0.00044415254,0.0007689906,0.00026507155,0.0003576988,0.00080590235],"category_scores_gemma":[0.0003044713,0.0001228346,0.00021624325,0.00052646355,0.0002524049,0.00031397486,0.000888346,0.00025460435,0.00023588986],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002735289,0.00015622974,0.7834299,0.00017166401,0.00015057402,0.007433131,0.0009788204,0.0010653948,0.16834472,0.0014111671,0.00074468885,0.03584012],"study_design_scores_gemma":[0.000013681692,0.00016467055,0.98022205,0.000029704612,0.000050826475,0.002889641,0.00048131574,0.0027377834,0.004238417,0.0004177956,0.008737781,0.000016323012],"about_ca_topic_score_codex":0.0038662732,"about_ca_topic_score_gemma":0.014113156,"teacher_disagreement_score":0.0038662732,"about_ca_system_score_codex":0.00033249773,"about_ca_system_score_gemma":0.00025130511,"threshold_uncertainty_score":0.0076875687},"labels":[],"label_agreement":null},{"id":"W2170495147","doi":"10.1088/0004-637x/729/1/60","title":"QUARK-NOVAE IN LOW-MASS X-RAY BINARIES WITH MASSIVE NEUTRON STARS: A UNIVERSAL MODEL FOR SHORT-HARD GAMMA-RAY BURSTS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Circumbinary planet; Neutron star; Ejecta; White dwarf; Gamma-ray burst; Accretion (finance); Compact star; X-ray binary","score_opus":0.020720264693313027,"score_gpt":0.22420355365267478,"score_spread":0.20348328895936174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2170495147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9619194,0.00041446486,0.029752003,0.00024019823,0.000028722628,0.000033109205,0.000102770064,0.00018098239,0.0073283785],"genre_scores_gemma":[0.99635565,0.00018029504,0.0018245626,0.000030853174,0.00002732181,0.00001795782,0.000055296467,0.000027938615,0.0014801723],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998332,0.000037070215,0.000011241397,0.000037032332,0.0000295651,0.000051846324],"domain_scores_gemma":[0.9993223,0.00014253381,0.00022753414,0.00007529437,0.000043176475,0.0001892521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048783503,0.0006254534,0.00066820864,0.0007080714,0.00088990404,0.0017740652,0.0012688659,0.001263368,0.0017820845],"category_scores_gemma":[0.0012685753,0.00029851036,0.00075066375,0.0004445011,0.0012724804,0.0016499261,0.0014775243,0.00053254643,0.00048247704],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007182,0.0005306506,0.23608819,0.00017973229,0.00020910123,0.005556548,0.0016993057,0.29493457,0.025645262,0.41153753,0.0018257388,0.021075154],"study_design_scores_gemma":[0.00008772268,0.00015472008,0.027283771,0.000030896248,0.000059134927,0.0015754516,0.00027563592,0.86400986,0.0009815638,0.10387238,0.0016137785,0.00005515694],"about_ca_topic_score_codex":0.0033223869,"about_ca_topic_score_gemma":0.002145787,"teacher_disagreement_score":0.0033223869,"about_ca_system_score_codex":0.0007010297,"about_ca_system_score_gemma":0.00036083526,"threshold_uncertainty_score":0.006606102},"labels":[],"label_agreement":null},{"id":"W2170555883","doi":"10.1088/0004-637x/800/1/59","title":"CHARACTERIZING K2 PLANET DISCOVERIES: A SUPER-EARTH TRANSITING THE BRIGHT K DWARF HIP 116454","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Saint Mary's University; Cape Breton University; University of Toronto; St. Mary's University; University of British Columbia","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Fundação para a Ciência e a Tecnologia; Smithsonian Astrophysical Observatory; Office of Science; Instituto de Astrofísica de Canarias; Université de Genève; European Commission; Science and Technology Facilities Council; University of St Andrews; Carnegie Mellon University; Scottish Universities Physics Alliance; Istituto Nazionale di Astrofisica; York University; University of Arizona; College of Engineering, Michigan State University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Harvard University; Austrian Science Fund; Ohio State University; National Geographic Society; U.S. Department of Energy; John Templeton Foundation; Smithsonian Institution; National Aeronautics and Space Administration; Space Telescope Science Institute; W. M. Keck Foundation; California Institute of Technology; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; National Science Foundation","keywords":"Planet; Transit (satellite); Photometry (optics); Spectrograph; Radial velocity; Proper motion; Planetary system; Population","score_opus":0.0180973733239766,"score_gpt":0.21967273356751213,"score_spread":0.20157536024353553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2170555883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99704605,0.00015561914,0.00037632638,0.000052662726,0.000015039881,0.000015506292,0.0006690524,0.00007025485,0.0015994313],"genre_scores_gemma":[0.99461997,0.00010361087,0.0016015628,0.00006656515,0.000026879728,0.000009564832,0.0027897048,0.000039267863,0.0007428171],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999713,0.000014614849,0.0000141883565,0.000081240585,0.000093022056,0.00008388196],"domain_scores_gemma":[0.9994954,0.000027730213,0.00013045028,0.00006312888,0.00011104289,0.000172277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030037283,0.0003178868,0.00025245183,0.0011241318,0.00088089827,0.0007112785,0.00039237697,0.00037578377,0.000466889],"category_scores_gemma":[0.00060081005,0.00020300901,0.0002032207,0.00062170386,0.00031418056,0.00036883954,0.0013577673,0.0003903107,0.00042013964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068197923,0.0001777028,0.8649731,0.00016385588,0.0001292491,0.005923661,0.0017715659,0.0009351807,0.09015225,0.0005291517,0.004071113,0.030491143],"study_design_scores_gemma":[0.00001799286,0.00026584484,0.975244,0.000024340228,0.000054863216,0.002504779,0.00071035733,0.0018278674,0.009263756,0.00017080773,0.00988461,0.000030786425],"about_ca_topic_score_codex":0.011618873,"about_ca_topic_score_gemma":0.023367148,"teacher_disagreement_score":0.011618873,"about_ca_system_score_codex":0.00049762434,"about_ca_system_score_gemma":0.00038251956,"threshold_uncertainty_score":0.023102522},"labels":[],"label_agreement":null},{"id":"W2170623042","doi":"10.1086/339350","title":"Evolution, Structure, and Seismology of Intermediate‐Mass Stars","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Asteroseismology; Oscillation (cell signaling); Astrophysics; Mixing (physics); Stellar evolution; Stellar structure; Stars; Stellar mass; Spectral line; Envelope (radar); Convection; Mass spectrum; Astronomy; Star formation; Mechanics; Mass spectrometry","score_opus":0.008010038683734115,"score_gpt":0.2030622214045683,"score_spread":0.1950521827208342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2170623042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950781,0.0007020574,0.00075893017,0.000071403694,0.0000043099694,0.000003252194,0.00017406729,0.00002999837,0.0031778677],"genre_scores_gemma":[0.99896955,0.00018974706,0.00026346356,0.000007005182,0.0000074071363,0.0000010774777,0.00024158983,0.0000050249705,0.00031525578],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99997103,0.000004197906,0.000002480535,0.000008599755,0.0000074660406,0.000006191608],"domain_scores_gemma":[0.99982893,0.000019148933,0.000059100712,0.000012906425,0.000037907186,0.00004195303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013198672,0.00010916016,0.00008126978,0.00078879413,0.00015354439,0.0003546273,0.000116588904,0.0001798458,0.00051509234],"category_scores_gemma":[0.00072287495,0.00008312622,0.000092224276,0.00041549795,0.00019010638,0.0002230256,0.00031706653,0.00017024876,0.00014950744],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021980904,0.000038521863,0.89901835,0.000051299307,0.000050554296,0.0005394165,0.0013499286,0.0032986973,0.038043655,0.004496034,0.0005078772,0.052385945],"study_design_scores_gemma":[0.0000045104894,0.00003761637,0.9950163,0.000007633503,0.0000117107165,0.00036902388,0.00010249304,0.0017897286,0.00052402046,0.0008477902,0.0012845342,0.0000046477558],"about_ca_topic_score_codex":0.0024091408,"about_ca_topic_score_gemma":0.0023345684,"teacher_disagreement_score":0.0024091408,"about_ca_system_score_codex":0.00024286579,"about_ca_system_score_gemma":0.00008800257,"threshold_uncertainty_score":0.0047902465},"labels":[],"label_agreement":null},{"id":"W2170931513","doi":"10.1086/317817","title":"Boomerang Returns Unexpectedly","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Cosmic microwave background; Universe; Cosmology; Scrutiny; Coherence (philosophical gambling strategy); Anisotropy; Cosmic background radiation","score_opus":0.005374746486827912,"score_gpt":0.23158195880409127,"score_spread":0.22620721231726335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2170931513","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04209211,0.008838621,0.0032291855,0.1546633,0.019890638,0.000054330638,0.0025456124,0.0013459189,0.7673403],"genre_scores_gemma":[0.24866325,0.0026318084,0.0011396148,0.034265548,0.003705494,0.000029422617,0.0011133517,0.00095259893,0.70749885],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99938524,0.00007802631,0.000014796366,0.00014104466,0.0001668813,0.0002139386],"domain_scores_gemma":[0.99874395,0.00019718142,0.00009715986,0.00022222855,0.00026789808,0.00047157277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00086603337,0.00053106254,0.00033090994,0.0008649419,0.0026869948,0.004004019,0.0005046721,0.0016521966,0.09077058],"category_scores_gemma":[0.004819794,0.00019198003,0.0002876398,0.00066331256,0.0022494968,0.0022443624,0.0022172271,0.0034189394,0.032972276],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002181447,0.00004673703,0.003175381,0.0000587063,0.00002503152,0.0010593081,0.00050900667,0.000104995794,0.00051188114,0.19246617,0.7077714,0.09405318],"study_design_scores_gemma":[0.000007560206,0.000020555399,0.002710358,0.000028167422,0.0000038367743,0.0003367321,0.00015026028,0.00008838993,0.00025408968,0.012500144,0.98389024,0.000009643727],"about_ca_topic_score_codex":0.006990394,"about_ca_topic_score_gemma":0.0140257925,"teacher_disagreement_score":0.09077058,"about_ca_system_score_codex":0.0013566073,"about_ca_system_score_gemma":0.0010124688,"threshold_uncertainty_score":0.30365783},"labels":[],"label_agreement":null},{"id":"W2171032444","doi":"10.1086/432246","title":"Microlensing Optical Depth toward the Galactic Bulge Using Clump Giants from the MACHO Survey","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Gravitational microlensing; Bulge; Astrophysics; Physics; Optical depth; Stars; Red clump; Astronomy; Giant star","score_opus":0.03398414336447562,"score_gpt":0.2590854005816957,"score_spread":0.2251012572172201,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171032444","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998664,0.00014618148,0.00024468396,0.0000110564715,0.0000014056861,0.0000035551805,0.00038755077,0.00001636358,0.0005251814],"genre_scores_gemma":[0.9984945,0.000090895126,0.00045240688,0.000009431118,0.0000068629724,0.000004190836,0.0008381705,0.0000047812814,0.00009873566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998375,0.000015884125,0.000007677882,0.00005465292,0.00003537965,0.00004894699],"domain_scores_gemma":[0.9992174,0.00012847761,0.0003016894,0.00007160696,0.00009294234,0.0001879031],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002966249,0.0002851292,0.00027154371,0.0017699552,0.00024610164,0.0005522433,0.00021093554,0.00022281242,0.0005803013],"category_scores_gemma":[0.0010621308,0.00017967491,0.00025603914,0.0007191847,0.00019020356,0.00035292326,0.0006753332,0.0002053201,0.00013196822],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012458091,0.000011638376,0.9841807,0.000021198019,0.000043509535,0.00009227611,0.00026,0.00037639035,0.0073275585,0.000088555,0.00014225523,0.0073312814],"study_design_scores_gemma":[0.0000036306424,0.000018733923,0.99847645,0.000004865913,0.000009104317,0.00008986179,0.000044712444,0.00060060737,0.00045874657,0.00003725373,0.00025210797,0.000003950444],"about_ca_topic_score_codex":0.006755713,"about_ca_topic_score_gemma":0.011301456,"teacher_disagreement_score":0.006755713,"about_ca_system_score_codex":0.00041537438,"about_ca_system_score_gemma":0.00012721906,"threshold_uncertainty_score":0.013432801},"labels":[],"label_agreement":null},{"id":"W2171046537","doi":"10.1088/0004-637x/720/2/1225","title":"THE ACS LCID PROJECT. III. THE STAR FORMATION HISTORY OF THE CETUS dSph GALAXY: A POST-REIONIZATION FOSSIL","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":184,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Reionization; Physics; Astrophysics; Milky Way; Galaxy; Astronomy; Dwarf galaxy; Local Group; Globular cluster; Star formation; Galaxy formation and evolution; Stars; Redshift","score_opus":0.006620538552397877,"score_gpt":0.198433848986925,"score_spread":0.19181331043452712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171046537","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.017299602,0.0005049863,0.007040667,0.00041602473,0.0001681992,0.0003199038,0.92080003,0.03010088,0.02334968],"genre_scores_gemma":[0.039725758,0.00033906323,0.031278085,0.00040092217,0.00013396617,0.0007831527,0.9144758,0.0034507064,0.009412543],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9994024,0.000056387067,0.000039045142,0.00013708665,0.0002822073,0.000082748564],"domain_scores_gemma":[0.99816126,0.00015263163,0.0002864369,0.0005430902,0.00053610944,0.00032056504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012135699,0.0011753389,0.0006940131,0.0050508194,0.0005245416,0.0022489438,0.0018812813,0.0005349146,0.01665654],"category_scores_gemma":[0.0026579266,0.00049747113,0.0006259585,0.005166555,0.0002262218,0.0013118272,0.0023144193,0.0006972791,0.021272106],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040815992,0.00012285502,0.039706156,0.00040671352,0.00014735293,0.00019112765,0.00039405687,0.000918225,0.0029414182,0.006450952,0.8773911,0.07092175],"study_design_scores_gemma":[0.00035898483,0.00004179501,0.08787842,0.000109145585,0.00008555732,0.0001418978,0.0002785913,0.0068767676,0.005240812,0.0052088797,0.89373237,0.000046773206],"about_ca_topic_score_codex":0.038748562,"about_ca_topic_score_gemma":0.029220376,"teacher_disagreement_score":0.038748562,"about_ca_system_score_codex":0.0013578198,"about_ca_system_score_gemma":0.0012366145,"threshold_uncertainty_score":0.07704604},"labels":[],"label_agreement":null},{"id":"W2171345686","doi":"10.1088/0004-637x/716/2/929","title":"LARGE-SCALE PERIODIC VARIABILITY OF THE WIND OF THE WOLF-RAYET STAR WR 1 (HD 4004)","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec; Natural Sciences and Engineering Research Council of Canada","funders":"","keywords":"Photometry (optics); Stars; Atmospheric dynamics; Coherence (philosophical gambling strategy); Rotation period; Spectroscopy; Be star; Stellar rotation; Emission spectrum","score_opus":0.005674324176231351,"score_gpt":0.20705136429538745,"score_spread":0.2013770401191561,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171345686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99936885,0.00001866357,0.000063086096,0.0000075020585,0.0000015180212,0.0000026387295,0.0002356172,0.0000074305135,0.00029470443],"genre_scores_gemma":[0.99836797,0.000026301817,0.00026538878,0.0000045539327,0.000007767977,0.000005614493,0.0010496,0.0000051682314,0.0002677022],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999292,0.000009686797,0.0000037938455,0.000021799471,0.00001756111,0.000018036893],"domain_scores_gemma":[0.9997669,0.000028966435,0.00008889743,0.000026468602,0.0000256123,0.000063180174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014509614,0.00016777731,0.00014455758,0.0005583482,0.00023428342,0.00029764444,0.00023747695,0.00019185762,0.0008745793],"category_scores_gemma":[0.00044965203,0.000083716805,0.00013052911,0.00037247362,0.00013473866,0.00018283968,0.00028600043,0.00018534606,0.00021945733],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043125814,0.00026458848,0.88663596,0.000052656524,0.00013206388,0.00070947467,0.0003146848,0.003208756,0.089641586,0.00029445396,0.0007211502,0.017593414],"study_design_scores_gemma":[0.000007846467,0.00007706707,0.9962053,0.0000021122287,0.000010395862,0.00010319738,0.000045422068,0.0018385111,0.0011606014,0.000053989297,0.000491159,0.000004487797],"about_ca_topic_score_codex":0.002955429,"about_ca_topic_score_gemma":0.003952423,"teacher_disagreement_score":0.002955429,"about_ca_system_score_codex":0.00028546868,"about_ca_system_score_gemma":0.00008727084,"threshold_uncertainty_score":0.0058764815},"labels":[],"label_agreement":null},{"id":"W2171539518","doi":"10.1088/0004-637x/730/2/81","title":"<i>CHANDRA</i>X-RAY OBSERVATIONS OF 12 MILLISECOND PULSARS IN THE GLOBULAR CLUSTER M28","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; University of Alberta; University of British Columbia; McGill University","funders":"","keywords":"Physics; Pulsar; Astrophysics; Globular cluster; Millisecond pulsar; Astronomy; X-ray pulsar; Luminosity; Neutron star; Galaxy; Observatory","score_opus":0.03575936143918136,"score_gpt":0.2906964922706741,"score_spread":0.2549371308314928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171539518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99780923,0.000088750785,0.00008963002,0.000028720951,0.0000026113853,0.000009348796,0.00065054,0.000033091397,0.0012880759],"genre_scores_gemma":[0.99547595,0.00017411097,0.0014340272,0.00004181087,0.00002724902,0.000018216515,0.0018801225,0.000017733746,0.00093081867],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999267,0.0000045268175,0.0000045292013,0.000017120337,0.000024053912,0.000023027564],"domain_scores_gemma":[0.99970055,0.000021798873,0.000071998096,0.00004367284,0.00004042607,0.00012158888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000119391545,0.00027042578,0.00023386051,0.0012887709,0.0003909602,0.000335701,0.00042145394,0.0001700651,0.001537625],"category_scores_gemma":[0.00033085633,0.0001711069,0.00015100969,0.0006539442,0.00015381622,0.0002654228,0.0007465709,0.00025101632,0.00031455487],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011075961,0.00033498506,0.7479356,0.00019294319,0.00015555626,0.0018226566,0.0013353592,0.0016211668,0.20223814,0.0005091644,0.0038094523,0.038937278],"study_design_scores_gemma":[0.000049838625,0.0001454522,0.99109155,0.000013053922,0.000020578853,0.0006679772,0.0001454214,0.0006335014,0.0038882385,0.000099347984,0.0032319725,0.000013120783],"about_ca_topic_score_codex":0.0055100634,"about_ca_topic_score_gemma":0.012695175,"teacher_disagreement_score":0.0055100634,"about_ca_system_score_codex":0.00026278745,"about_ca_system_score_gemma":0.00019038227,"threshold_uncertainty_score":0.010955989},"labels":[],"label_agreement":null},{"id":"W2171554667","doi":"10.1088/0004-637x/695/2/1430","title":"THE INHOMOGENEOUS BACKGROUND OF H<sub>2</sub>-DISSOCIATING RADIATION DURING COSMIC REIONIZATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; Background radiation; Galaxy; Radiative transfer; Starlight; Radiation; Stars; Dark Ages","score_opus":0.005290951981353817,"score_gpt":0.2013964812056376,"score_spread":0.1961055292242838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171554667","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98341656,0.00012750771,0.0071778926,0.00011920589,0.000018029901,0.000015248171,0.0005737546,0.00018436789,0.008367513],"genre_scores_gemma":[0.9976411,0.00006494398,0.0010886065,0.00003361274,0.000006197208,0.000011220603,0.0002632475,0.0000624764,0.00082868047],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991095,0.000021202324,0.0000030984047,0.000018840445,0.000016972037,0.000028921168],"domain_scores_gemma":[0.9995598,0.00016892079,0.00007800496,0.000050220286,0.00006184203,0.000081099795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026531832,0.00044950563,0.00029695028,0.0002574599,0.0003381288,0.0006680523,0.0008315084,0.00044174746,0.0015069778],"category_scores_gemma":[0.001364004,0.00026132783,0.0003520766,0.00048363995,0.00035607113,0.000505326,0.0003743057,0.0005023978,0.00020447474],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101414116,0.00005016998,0.023799999,0.000033155367,0.000044572684,0.00016047736,0.00006802015,0.9628638,0.0063129733,0.0037297693,0.0003386616,0.0024971624],"study_design_scores_gemma":[0.00004400473,0.000058070735,0.017975941,0.0000063701787,0.000026783007,0.00006393199,0.000054441032,0.97483,0.004488547,0.0016950807,0.0007379931,0.000018856745],"about_ca_topic_score_codex":0.014061935,"about_ca_topic_score_gemma":0.0071297144,"teacher_disagreement_score":0.014061935,"about_ca_system_score_codex":0.0010446984,"about_ca_system_score_gemma":0.00053884776,"threshold_uncertainty_score":0.027960181},"labels":[],"label_agreement":null},{"id":"W2171647268","doi":"10.1086/518762","title":"A New Population of High‐Redshift Short‐Duration Gamma‐Ray Bursts","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Redshift; Galaxy; Gamma-ray burst; Afterglow; Population; Photometric redshift","score_opus":0.010087165183172741,"score_gpt":0.24236939384300338,"score_spread":0.23228222865983064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171647268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99627364,0.00024224792,0.0019088141,0.000057178662,0.00001833664,0.000012983294,0.00010964318,0.00004778859,0.001329466],"genre_scores_gemma":[0.99617213,0.00022939645,0.0013764877,0.00009833031,0.0000893254,0.000018368322,0.0006503673,0.00002493769,0.0013406858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995172,0.000037419242,0.00003938436,0.00018072163,0.00013935537,0.00008581203],"domain_scores_gemma":[0.99850047,0.0002200629,0.00042880073,0.00035502482,0.00022539459,0.0002702234],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006941659,0.00026006022,0.00037415713,0.0012925485,0.0005779554,0.0017348,0.00073483336,0.0004059221,0.0016794036],"category_scores_gemma":[0.0015911789,0.0003034223,0.00025068317,0.0008426528,0.00062670466,0.0008487849,0.0008463225,0.0006611295,0.00050165964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026733315,0.00009678916,0.9392014,0.000028286664,0.000058019992,0.00082047476,0.0011743,0.0003270754,0.023874456,0.001808057,0.00072534295,0.031618427],"study_design_scores_gemma":[0.000038366437,0.00023485131,0.9732197,0.000015449257,0.00003881654,0.012484105,0.0005749431,0.0021170499,0.002205229,0.0017519037,0.007283796,0.000035805373],"about_ca_topic_score_codex":0.0010777182,"about_ca_topic_score_gemma":0.0015886939,"teacher_disagreement_score":0.0017348,"about_ca_system_score_codex":0.0003095138,"about_ca_system_score_gemma":0.00016932581,"threshold_uncertainty_score":0.0056180954},"labels":[],"label_agreement":null},{"id":"W2171708974","doi":"10.1086/427902","title":"Gemini Multi-Object Spectrograph Integral Field Spectroscopy of a Merging System with Enhanced Balmer Absorption","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Balmer series; Astrophysics; Galaxy; Population; Stars; Star formation; Integral field spectrograph; Astronomy; Spectral line; Spectrograph; Emission spectrum","score_opus":0.005170222281175807,"score_gpt":0.21785693892349725,"score_spread":0.21268671664232144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171708974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881494,0.00005033053,0.00034563194,0.000034186804,0.000001958266,0.0000049759838,0.00017609855,0.00004706037,0.0005248805],"genre_scores_gemma":[0.9975043,0.000027835402,0.0016715457,0.000022507147,0.0000052872533,0.0000030385345,0.00057382334,0.000009744475,0.00018190422],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999124,0.000009878118,0.0000049738705,0.000021330492,0.000025148853,0.000026234049],"domain_scores_gemma":[0.9997867,0.000011252372,0.000073845295,0.0000245173,0.000024733828,0.00007884863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025651438,0.00021009592,0.00016612351,0.0007400192,0.00046455258,0.00039994236,0.0002144221,0.00018820236,0.00055956986],"category_scores_gemma":[0.00025951207,0.0001405333,0.00017047489,0.0007420432,0.00016446781,0.00036668743,0.0004660508,0.00018247044,0.00016380173],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002725996,0.0001532462,0.8840011,0.000029100422,0.000073126925,0.0008068121,0.0007742945,0.001945892,0.08972089,0.0005198439,0.0012792086,0.020423867],"study_design_scores_gemma":[0.0000084034455,0.00004581538,0.9922501,0.0000023627197,0.000018071489,0.0002273647,0.00018073221,0.0039150515,0.0021467037,0.00012118821,0.0010780431,0.0000062407366],"about_ca_topic_score_codex":0.0081719365,"about_ca_topic_score_gemma":0.016317327,"teacher_disagreement_score":0.0081719365,"about_ca_system_score_codex":0.00045034694,"about_ca_system_score_gemma":0.00018871951,"threshold_uncertainty_score":0.016248763},"labels":[],"label_agreement":null},{"id":"W2171758905","doi":"10.1088/0004-637x/792/2/102","title":"ESTIMATING LUMINOSITIES AND STELLAR MASSES OF GALAXIES PHOTOMETRICALLY WITHOUT DETERMINING REDSHIFTS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Photometry (optics); Galaxy; Redshift; Luminosity; Photometric redshift; Stellar mass; Surface brightness fluctuation; Luminous infrared galaxy","score_opus":0.008807928437804115,"score_gpt":0.22462282733777997,"score_spread":0.21581489889997585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171758905","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5384208,0.00044849783,0.44389594,0.00015940255,0.000032177806,0.00008783397,0.0026389495,0.010209273,0.004107094],"genre_scores_gemma":[0.78205585,0.00014529216,0.20968084,0.00009290127,0.00003604897,0.0000668994,0.0063316743,0.0006241532,0.00096634415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99911684,0.00014755598,0.000047206722,0.00037735858,0.00024129571,0.00006978298],"domain_scores_gemma":[0.99728346,0.00043690178,0.0005170155,0.001283958,0.00037510158,0.000103541744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014557629,0.00094094564,0.0007614539,0.0026468313,0.0004865758,0.0013530157,0.0014874628,0.0010143274,0.0011913617],"category_scores_gemma":[0.008121504,0.0009376683,0.00107133,0.0018999198,0.0005095267,0.0013901759,0.0012707065,0.000826692,0.0015642227],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019592045,0.00035187573,0.48400298,0.00023686509,0.00058671157,0.0001273209,0.00038094324,0.14437656,0.0525898,0.00574933,0.0043699523,0.30703172],"study_design_scores_gemma":[0.00006259712,0.0000661609,0.35199514,0.00005624972,0.00011159708,0.00033794343,0.00011175843,0.59271544,0.0409627,0.0067188307,0.006779601,0.00008204604],"about_ca_topic_score_codex":0.006143566,"about_ca_topic_score_gemma":0.007611328,"teacher_disagreement_score":0.006143566,"about_ca_system_score_codex":0.0009361053,"about_ca_system_score_gemma":0.00053894613,"threshold_uncertainty_score":0.012215614},"labels":[],"label_agreement":null},{"id":"W2171811285","doi":"10.1088/0004-637x/787/2/137","title":"ARECIBO PULSAR SURVEY USING ALFA. III. PRECURSOR SURVEY AND POPULATION SYNTHESIS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Science Foundation","keywords":"Millisecond pulsar; Pulsar; Galactic plane; Millisecond; Observable","score_opus":0.030012699548166426,"score_gpt":0.3270068028400685,"score_spread":0.29699410329190207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171811285","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.726795,0.00051950285,0.020021955,0.00022509503,0.000080700134,0.0029280174,0.18728457,0.001844376,0.060300797],"genre_scores_gemma":[0.56082356,0.0009780286,0.052533213,0.0002994039,0.00012581733,0.004231326,0.35508236,0.00034330084,0.025582982],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999765,0.000050084127,0.000013430916,0.00006372187,0.00006684481,0.00004086255],"domain_scores_gemma":[0.99960035,0.000036984748,0.00008684436,0.00008542429,0.00014784295,0.000042560092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003905964,0.00031846616,0.00025178023,0.002398024,0.0002873898,0.00040980356,0.00042153048,0.00013806016,0.007108935],"category_scores_gemma":[0.0010373737,0.00019035216,0.00029856613,0.0017317999,0.00009782289,0.00013883907,0.00041138608,0.00019027211,0.0029534232],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00075022713,0.00027363416,0.6457327,0.00028481113,0.00020156804,0.00031296705,0.0005511557,0.0051217945,0.013500413,0.0047102445,0.078826785,0.24973375],"study_design_scores_gemma":[0.00012074496,0.000109675,0.895999,0.000030296696,0.00004561482,0.00018424458,0.0002041653,0.0046106894,0.0013966118,0.00066441024,0.09661976,0.00001480052],"about_ca_topic_score_codex":0.046940964,"about_ca_topic_score_gemma":0.04647097,"teacher_disagreement_score":0.046940964,"about_ca_system_score_codex":0.00047127678,"about_ca_system_score_gemma":0.0007193225,"threshold_uncertainty_score":0.09333545},"labels":[],"label_agreement":null},{"id":"W2171896719","doi":"10.1088/0004-637x/738/1/48","title":"X-RAY PROPERTIES OF THE FIRST SUNYAEV-ZEL'DOVICH EFFECT SELECTED GALAXY CLUSTER SAMPLE FROM THE SOUTH POLE TELESCOPE","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":179,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Kavli Institute for Cosmological Physics, University of Chicago; University of Chicago; Smithsonian Astrophysical Observatory; McGill University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Gordon and Betty Moore Foundation; W. M. Keck Foundation; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; Cosmic microwave background; Astrophysics; Galaxy cluster; Sunyaev–Zel'dovich effect; South Pole Telescope; Intracluster medium; Scaling; Cluster (spacecraft); Normalization (sociology); Telescope; Galaxy; Anisotropy; Geometry","score_opus":0.009869156701326175,"score_gpt":0.18107049480233436,"score_spread":0.17120133810100818,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2171896719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988998,0.000028455552,0.00003007134,0.0000068631143,5.545865e-7,0.0000035198975,0.00076447637,0.0000067527044,0.00025943803],"genre_scores_gemma":[0.996449,0.000033873956,0.00009043347,0.000007825524,0.0000033589536,0.000007101003,0.0030294613,0.0000074952495,0.0003714013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998398,0.000010241881,0.000006701868,0.000048707105,0.000045244153,0.000049241502],"domain_scores_gemma":[0.999366,0.00007284998,0.00019386926,0.00007424164,0.00006778692,0.00022533021],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017330519,0.0002629343,0.00035499755,0.0012446744,0.00046824367,0.0005200895,0.00024513868,0.0001682902,0.0014497126],"category_scores_gemma":[0.00040500314,0.00016169483,0.00018889883,0.00074319955,0.00025412222,0.00015953089,0.00054789224,0.00020066524,0.0003497394],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014574334,0.00003593179,0.9911442,0.000013784911,0.000052858843,0.0000986669,0.0002852096,0.0004310859,0.0047114263,0.000076216755,0.0007017845,0.0023031177],"study_design_scores_gemma":[0.000003939274,0.00001338336,0.999328,7.822262e-7,0.0000051339216,0.00003275512,0.000039610724,0.00012242982,0.0001879212,0.000005616051,0.00025891635,0.0000014602708],"about_ca_topic_score_codex":0.01447256,"about_ca_topic_score_gemma":0.02758059,"teacher_disagreement_score":0.01447256,"about_ca_system_score_codex":0.0004701165,"about_ca_system_score_gemma":0.0001867749,"threshold_uncertainty_score":0.028776646},"labels":[],"label_agreement":null},{"id":"W2172064654","doi":"10.1088/0004-637x/764/1/73","title":"ON THE ORIGIN OF MASS SEGREGATION IN NGC 3603","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Astronomy; Stellar wind; Stars","score_opus":0.012248365819907151,"score_gpt":0.22220772637643718,"score_spread":0.20995936055653003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2172064654","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987263,0.00010446665,0.00018925579,0.00002838478,0.0000022544448,0.0000014155313,0.000111762136,0.000030209132,0.0008060126],"genre_scores_gemma":[0.9995142,0.000027270706,0.00013316302,0.000008688895,0.0000019958534,0.0000011287686,0.00019222568,0.0000074085956,0.000113892],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998503,0.000012241536,0.000009304837,0.00004994516,0.000040940067,0.000037365513],"domain_scores_gemma":[0.9995702,0.00005261495,0.00018003983,0.00004262579,0.00006407187,0.00009045402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001789411,0.00022767483,0.00022473498,0.0013669789,0.00067341764,0.00061125786,0.00033573818,0.00033380982,0.0010734177],"category_scores_gemma":[0.0006329556,0.00014932679,0.0002117668,0.0008226438,0.0006455812,0.0002399475,0.000603092,0.00022179185,0.00042691742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020977994,0.00001720375,0.948704,0.00001928773,0.000023564666,0.00042815664,0.0009422591,0.0006803333,0.0393149,0.0006460895,0.0003249021,0.008689327],"study_design_scores_gemma":[0.0000029920045,0.00001796251,0.99666435,0.000006390928,0.0000074581976,0.00021153496,0.00021023155,0.0007152666,0.0011863586,0.00029773827,0.0006739055,0.0000059153963],"about_ca_topic_score_codex":0.016408296,"about_ca_topic_score_gemma":0.01969693,"teacher_disagreement_score":0.016408296,"about_ca_system_score_codex":0.0009217374,"about_ca_system_score_gemma":0.00020668501,"threshold_uncertainty_score":0.032625556},"labels":[],"label_agreement":null},{"id":"W2172108351","doi":"10.1086/427390","title":"TeV Emission from the Galactic Center Black Hole Plerion","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Galactic Center; Fermi acceleration; Electron; Pulsar; Magnetohydrodynamics; Accretion (finance); Synchrotron radiation; Fermi Gamma-ray Space Telescope; Black hole (networking)","score_opus":0.013266311485149281,"score_gpt":0.2317876620164307,"score_spread":0.2185213505312814,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2172108351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99169195,0.0008365505,0.00042805166,0.00016080987,0.000027350494,0.0000148613735,0.00041693708,0.00010721343,0.00631631],"genre_scores_gemma":[0.9978916,0.0002131057,0.00032671954,0.00018738052,0.000043096697,0.0000058769874,0.00046559973,0.000012313051,0.0008544062],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995494,0.000004393612,0.0000013742613,0.000017343695,0.000010382194,0.000011507724],"domain_scores_gemma":[0.9999256,0.000008189075,0.000029476078,0.000012159729,0.0000061189853,0.000018566003],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009941697,0.00022132437,0.00013587494,0.00046994266,0.0002633701,0.00040462744,0.00017066501,0.00035414926,0.0011050964],"category_scores_gemma":[0.00013246622,0.00011603569,0.00015967713,0.00023465634,0.0001842557,0.00010024012,0.00045504209,0.00025571248,0.00030618822],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011538437,0.000100372956,0.4698522,0.00021776595,0.00019283034,0.011457323,0.0012979958,0.00020140086,0.46369818,0.0010622675,0.005701674,0.045064166],"study_design_scores_gemma":[0.000029438455,0.00024704408,0.9737376,0.000033842825,0.000046588728,0.004817912,0.0001637918,0.00026955866,0.012258633,0.00020672215,0.008175841,0.000013049813],"about_ca_topic_score_codex":0.00057917956,"about_ca_topic_score_gemma":0.00068869244,"teacher_disagreement_score":0.0011050964,"about_ca_system_score_codex":0.0001651618,"about_ca_system_score_gemma":0.000028128672,"threshold_uncertainty_score":0.0036969185},"labels":[],"label_agreement":null},{"id":"W2172169318","doi":"10.1088/0004-637x/798/1/26","title":"EVIDENCE FOR (AND AGAINST) PROGENITOR BIAS IN THE SIZE GROWTH OF COMPACT RED GALAXIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Toronto","funders":"","keywords":"Astrophysics; Physics; Elliptical galaxy; Galaxy; Astronomy; Bulge; Luminous infrared galaxy; Galaxy group","score_opus":0.03140799147547197,"score_gpt":0.25875583350061626,"score_spread":0.2273478420251443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2172169318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99887305,0.0001709557,0.0002732688,0.000043083994,0.0000028264158,0.0000016426371,0.000060844217,0.000009842766,0.0005644351],"genre_scores_gemma":[0.99962735,0.0000326179,0.000074798605,0.000019880596,0.0000068477198,9.152061e-7,0.00006915708,0.000003572524,0.00016492605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992879,0.00012412651,0.00005235012,0.0002789458,0.0001563585,0.0001003637],"domain_scores_gemma":[0.987457,0.0044990773,0.0042305663,0.0015480008,0.0010544893,0.0012108795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018611,0.00016534112,0.00029130728,0.001062068,0.0003125866,0.0011127557,0.000757903,0.0005524368,0.002334314],"category_scores_gemma":[0.005931733,0.00025755173,0.000239337,0.0005096224,0.0012890514,0.0008924629,0.0010475732,0.00038513358,0.00035210748],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026611504,0.00002313661,0.9829306,0.000024096198,0.000050356615,0.00006723503,0.0004620639,0.000107310814,0.00965906,0.0005112453,0.000065751985,0.0058330586],"study_design_scores_gemma":[0.000006585437,0.00004966241,0.99800783,0.000003714695,0.000016821186,0.0001313426,0.00016027219,0.00021141044,0.0010893858,0.00016789253,0.00015184224,0.000003392111],"about_ca_topic_score_codex":0.0017721859,"about_ca_topic_score_gemma":0.0027706942,"teacher_disagreement_score":0.002334314,"about_ca_system_score_codex":0.00026461575,"about_ca_system_score_gemma":0.00017995782,"threshold_uncertainty_score":0.009842515},"labels":[],"label_agreement":null},{"id":"W2172216553","doi":"10.1088/0004-637x/804/1/53","title":"A MEASUREMENT OF DIFFUSION IN 47 TUCANAE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"Globular cluster; Physics; Diffusion; Stars; Astrophysics; Advanced Camera for Surveys; White dwarf; Hubble space telescope; Relaxation (psychology); Astronomy; Medicine","score_opus":0.02575504806248412,"score_gpt":0.23167627747169753,"score_spread":0.2059212294092134,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2172216553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997071,0.00017973944,0.00048234628,0.000033066946,0.0000038308003,0.0000064799783,0.0003568391,0.000028944141,0.0018378675],"genre_scores_gemma":[0.9972957,0.00015615679,0.0010668423,0.000018952534,0.0000051579063,0.000011231918,0.0006083756,0.000014668419,0.00082292495],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998821,0.0000037799293,0.0000028628344,0.00004625654,0.000024326066,0.00004061161],"domain_scores_gemma":[0.9997148,0.000030843563,0.00007699145,0.000025053265,0.00008049558,0.00007184061],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001243479,0.00021914703,0.0002932624,0.0012811659,0.001041697,0.00067231443,0.00054086384,0.00057402765,0.0009631554],"category_scores_gemma":[0.0007351142,0.00020373675,0.00018511116,0.0010778793,0.00038891958,0.0004531369,0.00060822954,0.0004594436,0.00018916506],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005880089,0.00007167993,0.4466522,0.00009523364,0.00018822827,0.00024004505,0.0026071297,0.005311704,0.50517285,0.0022553531,0.0014162511,0.03540129],"study_design_scores_gemma":[0.000013538819,0.000037915877,0.97056985,0.000013084246,0.000044906148,0.00018995257,0.00035281965,0.00556167,0.019395113,0.00022607693,0.0035544108,0.00004058759],"about_ca_topic_score_codex":0.19096948,"about_ca_topic_score_gemma":0.18538211,"teacher_disagreement_score":0.19096948,"about_ca_system_score_codex":0.0023968436,"about_ca_system_score_gemma":0.000690324,"threshold_uncertainty_score":0.3797158},"labels":[],"label_agreement":null},{"id":"W2172286143","doi":"10.1088/0004-637x/736/2/117","title":"NEW OPTICAL/ULTRAVIOLET COUNTERPARTS AND THE SPECTRAL ENERGY DISTRIBUTIONS OF NEARBY, THERMALLY EMITTING, ISOLATED NEUTRON STARS","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Photometry (optics); Ultraviolet; Astrophysics; Stars; Neutron star; Spectral line; Spectral energy distribution; Wavelength; Astronomy; Optics","score_opus":0.009270027112476837,"score_gpt":0.2040406918125488,"score_spread":0.19477066470007195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2172286143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918896,0.000058462585,0.0001560701,0.000004893994,8.469441e-7,8.3921424e-7,0.00007089682,0.000006364827,0.0005128131],"genre_scores_gemma":[0.9992774,0.000030073039,0.0003667023,0.0000046118016,0.000005819171,0.0000011559615,0.00018976499,0.0000029661867,0.00012154425],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998994,0.000010106456,0.000011425116,0.00003557381,0.000026559606,0.000016918415],"domain_scores_gemma":[0.99921155,0.000087131826,0.00042463178,0.00007100459,0.00007198353,0.00013365546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027515998,0.00020491407,0.00014278473,0.0015968812,0.00028291444,0.0004283546,0.00021716412,0.00019082919,0.0009583443],"category_scores_gemma":[0.00052797515,0.00013109029,0.00012048397,0.00066183304,0.000275027,0.0002934755,0.00042224475,0.0001763218,0.00019943836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025194092,0.000033114276,0.9588572,0.000029627192,0.000036842146,0.00020362248,0.00030552142,0.00034139006,0.030590756,0.0003733889,0.000101034595,0.008875588],"study_design_scores_gemma":[0.0000040016034,0.000045923458,0.99637455,0.000004273124,0.00001720503,0.0004839674,0.00011844171,0.00047384683,0.0019575576,0.00020312781,0.00031306612,0.0000040557793],"about_ca_topic_score_codex":0.0006301753,"about_ca_topic_score_gemma":0.0017869931,"teacher_disagreement_score":0.0015968812,"about_ca_system_score_codex":0.00019081845,"about_ca_system_score_gemma":0.000048576614,"threshold_uncertainty_score":0.0032060146},"labels":[],"label_agreement":null},{"id":"W2174781540","doi":"10.3847/0004-637x/817/1/40","title":"DETERMINING AGES OF APOGEE GIANTS WITH KNOWN DISTANCES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Stars; Physics; Surface gravity; Astrophysics; Metallicity; Spectral line; Red-giant branch; Asymptotic giant branch; Astronomy","score_opus":0.010049640420723042,"score_gpt":0.22039780423796962,"score_spread":0.21034816381724658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2174781540","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99859434,0.00012442267,0.0005756232,0.000010111667,0.0000017782775,0.000003864595,0.0003194858,0.000019211315,0.00035117174],"genre_scores_gemma":[0.9987257,0.00005066259,0.0005257436,0.000008228053,0.0000027023798,0.0000045418346,0.0004588119,0.0000060998686,0.00021735425],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998053,0.000028452514,0.00001387984,0.000071879396,0.000049036422,0.00003160382],"domain_scores_gemma":[0.9986601,0.0003285713,0.0004108093,0.00016064633,0.00028962016,0.00015018492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006489157,0.00025095147,0.00028207386,0.0017796431,0.00032768206,0.0004851207,0.00030245766,0.00037416373,0.00087022857],"category_scores_gemma":[0.0023349246,0.00017305897,0.00019445979,0.000604275,0.000251713,0.0005396154,0.0005085408,0.00018510022,0.00051496836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004781329,0.0000054476304,0.99251235,0.0000078376925,0.000024385497,0.000046890196,0.00018100321,0.00047417165,0.0024623573,0.00006100716,0.00008428275,0.0040924735],"study_design_scores_gemma":[0.000002367399,0.000016496051,0.9974509,0.000003791845,0.000011048182,0.00007803139,0.00012318153,0.0010910854,0.00069078314,0.00008543511,0.00044269502,0.0000042251013],"about_ca_topic_score_codex":0.0051137,"about_ca_topic_score_gemma":0.009257218,"teacher_disagreement_score":0.0051137,"about_ca_system_score_codex":0.0004982259,"about_ca_system_score_gemma":0.00010345943,"threshold_uncertainty_score":0.010167837},"labels":[],"label_agreement":null},{"id":"W2174822282","doi":"10.3847/0004-637x/823/2/114","title":"SPECTROSCOPIC DETERMINATION OF MASSES (AND IMPLIED AGES) FOR RED GIANTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":209,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Office of Science; Max-Planck-Institut für Astronomie; National Science Foundation; Liverpool John Moores University; York University; Science and Technology Facilities Council; Carnegie Mellon University; Princeton University; Alfred P. Sloan Foundation; University of Washington; College of Engineering, Michigan State University; Johns Hopkins University; U.S. Department of Energy; Arizona State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Aeronautics and Space Administration; Brookhaven National Laboratory; European Commission","keywords":"Milky Way; Red giant; Stellar population; Stars; Red clump; Spectral line; Giant star; Red-giant branch","score_opus":0.012023874174632356,"score_gpt":0.24823440192410914,"score_spread":0.2362105277494768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2174822282","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9820318,0.001246594,0.0073360754,0.0001918585,0.000024516747,0.000015951024,0.0038608955,0.00041897356,0.0048732483],"genre_scores_gemma":[0.9895321,0.00037877832,0.0057101883,0.000052704214,0.000023855542,0.000012542511,0.0031898613,0.0000435229,0.0010564827],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998037,0.000022483342,0.000015001079,0.0000719316,0.000060277092,0.000026512047],"domain_scores_gemma":[0.99856913,0.00021420573,0.00057288085,0.00021190933,0.00031015294,0.000121721554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009428437,0.0002910838,0.00021015023,0.0029012566,0.0003527554,0.0006558257,0.00039003923,0.00044887495,0.0015819187],"category_scores_gemma":[0.0027864685,0.00019678177,0.00021717304,0.0012228335,0.00022648618,0.00055135525,0.0006681749,0.00020616934,0.0009844037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008786182,0.000014114527,0.9506211,0.00006833966,0.000038592287,0.000085444546,0.00030815045,0.0010555818,0.014673652,0.0017280482,0.002002925,0.02931624],"study_design_scores_gemma":[0.000006574579,0.000036316083,0.97961104,0.000038697664,0.000036047284,0.0003088631,0.00019275752,0.005334048,0.0051586404,0.0020367233,0.007223384,0.000017006274],"about_ca_topic_score_codex":0.002186502,"about_ca_topic_score_gemma":0.004202228,"teacher_disagreement_score":0.0029012566,"about_ca_system_score_codex":0.0004921199,"about_ca_system_score_gemma":0.00016018373,"threshold_uncertainty_score":0.0052919984},"labels":[],"label_agreement":null},{"id":"W2176245720","doi":"10.3847/0004-637x/817/1/20","title":"A POPULATION OF INTERMEDIATE-MASS BLACK HOLES IN DWARF STARBURST GALAXIES UP TO REDSHIFT = 1.5","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Redshift; Supermassive black hole; Galaxy; Population","score_opus":0.008358318609194004,"score_gpt":0.22449482613208033,"score_spread":0.21613650752288632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2176245720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998166,0.00003132622,0.000021356904,0.000008821914,6.657311e-7,9.389674e-7,0.00005254497,0.0000016624343,0.00006603279],"genre_scores_gemma":[0.99979264,0.000014351778,0.0000133291405,0.0000054556654,0.0000018022403,5.7350803e-7,0.000096577714,5.1690824e-7,0.00007489871],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978477,0.000024251847,0.0000108263375,0.00007766469,0.000029466952,0.00007309043],"domain_scores_gemma":[0.9991947,0.00009134797,0.00028342966,0.00006590556,0.00007101477,0.00029365887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003393966,0.00019557621,0.00023021526,0.0011954375,0.000456434,0.0007935892,0.00041829035,0.0002751062,0.0018108676],"category_scores_gemma":[0.000863055,0.00015860416,0.00018536656,0.0004950935,0.00045312828,0.0004254628,0.0004995298,0.00025460048,0.00031860312],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030181372,0.000015372372,0.99812454,0.000001932714,0.000008337378,0.000047361846,0.00019293277,0.000027194405,0.0005738476,0.000039546685,0.000031913474,0.00090680487],"study_design_scores_gemma":[0.0000018083433,0.000029265397,0.9993969,0.0000014968665,0.0000050678777,0.0001166685,0.000205165,0.00009314095,0.000057817153,0.00002481681,0.00006658839,0.0000012224084],"about_ca_topic_score_codex":0.005904771,"about_ca_topic_score_gemma":0.006523099,"teacher_disagreement_score":0.005904771,"about_ca_system_score_codex":0.00019774893,"about_ca_system_score_gemma":0.00012338434,"threshold_uncertainty_score":0.011740804},"labels":[],"label_agreement":null},{"id":"W2176989236","doi":"10.3847/0004-637x/816/2/75","title":"THE SEARCH FOR TRANSIENT ASTROPHYSICAL NEUTRINO EMISSION WITH ICECUBE-DEEPCORE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; U.S. Department of Energy; University of Wisconsin-Madison; Vetenskapsrådet; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; Vlaamse regering; University of Oxford; Compute Canada; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Neutrino; Supernova; Neutrino astronomy; Astrophysics; Neutrino detector; Muon neutrino; Astronomy; Point source; Astroparticle physics; Sky; Neutrino oscillation; Nuclear physics","score_opus":0.010463704651553633,"score_gpt":0.23338230340863608,"score_spread":0.22291859875708245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2176989236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9523202,0.00035150512,0.006715746,0.00016866815,0.000029460954,0.00011957522,0.030613426,0.0006029436,0.009078439],"genre_scores_gemma":[0.92458767,0.00016260693,0.018569518,0.00007862745,0.00003921601,0.00011344283,0.055403244,0.00016633022,0.00087932736],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99953747,0.000069386566,0.00001529754,0.00012525031,0.00014919574,0.00010350485],"domain_scores_gemma":[0.9986847,0.0003548659,0.00032905414,0.00023718902,0.00021824137,0.00017591091],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014672609,0.0004956956,0.00048197465,0.0015799678,0.00040456437,0.0008242944,0.0006056072,0.00029774205,0.0014667127],"category_scores_gemma":[0.0018016187,0.0002133893,0.0005388596,0.0020116437,0.00030817642,0.0004440302,0.0009961582,0.0004721626,0.0003287309],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0038554717,0.0005397147,0.795275,0.0002878426,0.000938137,0.00085389026,0.0004660945,0.051940013,0.058721397,0.007334028,0.019152636,0.06063591],"study_design_scores_gemma":[0.0003644246,0.0005384932,0.7957273,0.00007256823,0.00031405027,0.00072587404,0.0003283306,0.10125785,0.05195522,0.0038050225,0.044811048,0.00009979569],"about_ca_topic_score_codex":0.008817233,"about_ca_topic_score_gemma":0.015485564,"teacher_disagreement_score":0.008817233,"about_ca_system_score_codex":0.00074529456,"about_ca_system_score_gemma":0.00085852057,"threshold_uncertainty_score":0.017531812},"labels":[],"label_agreement":null},{"id":"W2179618759","doi":"10.3847/0004-637x/821/1/65","title":"EVIDENCE FOR REFLECTED LIGHT FROM THE MOST ECCENTRIC EXOPLANET KNOWN","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Exoplanet; Ephemeris; Orbital eccentricity; Astrometry; Planet; Photometry (optics); Radial velocity; Planetary system; Transit (satellite); Eccentricity (behavior)","score_opus":0.030189818459690456,"score_gpt":0.26326612396842086,"score_spread":0.2330763055087304,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2179618759","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926109,0.00009956235,0.00045729772,0.00007304186,0.00001050519,0.000007334239,0.00049948244,0.0000714201,0.0061704824],"genre_scores_gemma":[0.9981035,0.000032243006,0.00034992027,0.000040023304,0.000009182195,0.000003221416,0.00039992935,0.000012429767,0.001049518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981743,0.000018788623,0.000014041867,0.000049203692,0.0000564907,0.000044002045],"domain_scores_gemma":[0.99935967,0.000101209655,0.00016566084,0.0000815865,0.00012075218,0.00017106492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018385347,0.00017446597,0.00018099479,0.0012003428,0.00033660317,0.00040513556,0.00027974945,0.00038667137,0.004372241],"category_scores_gemma":[0.00051616674,0.00014983812,0.00015032239,0.00047620348,0.00021738726,0.00021761953,0.00033593219,0.00029640467,0.00097020296],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039292016,0.00012607983,0.8176031,0.000051243194,0.000055931527,0.0023019144,0.0006773508,0.00007979095,0.15911496,0.00036318577,0.0013969122,0.017836556],"study_design_scores_gemma":[0.000008205325,0.00019041808,0.982904,0.000008797506,0.000017744118,0.003411502,0.0002527318,0.0002593289,0.010106468,0.000085520616,0.0027480898,0.0000071648565],"about_ca_topic_score_codex":0.0011417047,"about_ca_topic_score_gemma":0.0020673384,"teacher_disagreement_score":0.004372241,"about_ca_system_score_codex":0.00021900499,"about_ca_system_score_gemma":0.00007286392,"threshold_uncertainty_score":0.014626622},"labels":[],"label_agreement":null},{"id":"W2181312162","doi":"10.3847/0004-637x/818/1/92","title":"THE NANOGRAV NINE-YEAR DATA SET: ASTROMETRIC MEASUREMENTS OF 37 MILLISECOND PULSARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"","keywords":"Millisecond pulsar; Physics; Pulsar; Astrophysics; Population; Astronomy; Proper motion; Parallax; Neutron star; Green Bank Telescope; Stars","score_opus":0.05419685408200407,"score_gpt":0.3418706933966991,"score_spread":0.28767383931469503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2181312162","genre_codex":"empirical","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96170175,0.00020416931,0.0021561142,0.00007489182,0.000035449004,0.000052077594,0.029879145,0.00019552608,0.005700883],"genre_scores_gemma":[0.888501,0.00020803,0.0077486,0.00009514947,0.00005544803,0.00012563684,0.101048954,0.00009251802,0.0021246192],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995338,0.000040911305,0.00004943885,0.00011309545,0.00022525739,0.000037594487],"domain_scores_gemma":[0.9979194,0.0002058181,0.00044999155,0.0005343667,0.00068380096,0.00020667075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069228205,0.00024758742,0.00027598103,0.0021534653,0.0003400753,0.00044771217,0.00045411932,0.00022775777,0.001101874],"category_scores_gemma":[0.0016362073,0.00016265373,0.00017542647,0.0022667279,0.0001723034,0.00045029735,0.0008508052,0.00030442924,0.00074642326],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028675207,0.00010639465,0.93884194,0.00007574083,0.00009700091,0.00014259544,0.00036166227,0.0013928311,0.017278284,0.00041564496,0.005741634,0.03525966],"study_design_scores_gemma":[0.000017610157,0.00004234315,0.98620033,0.000007042165,0.000018321782,0.00009003516,0.00006928747,0.0012708828,0.002125145,0.000079983896,0.010066333,0.000012810856],"about_ca_topic_score_codex":0.009063174,"about_ca_topic_score_gemma":0.023524214,"teacher_disagreement_score":0.009063174,"about_ca_system_score_codex":0.00032615144,"about_ca_system_score_gemma":0.00027198135,"threshold_uncertainty_score":0.018020868},"labels":[],"label_agreement":null},{"id":"W2182694480","doi":"10.3847/0004-637x/818/2/179","title":"EVIDENCE FOR THE RAPID FORMATION OF LOW-MASS EARLY-TYPE GALAXIES IN DENSE ENVIRONMENTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Galaxy; Virgo Cluster; RADIUS; Halo; Stars; Star formation; Elliptical galaxy; Virial theorem; Galaxy cluster","score_opus":0.018322933847004678,"score_gpt":0.23085266787497966,"score_spread":0.21252973402797498,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2182694480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995431,0.000035307552,0.00008965408,0.0000071495956,5.227736e-7,9.273177e-7,0.000033588298,0.000004907584,0.00028498884],"genre_scores_gemma":[0.9997564,0.000014208973,0.00007690108,0.000006715833,0.000001836735,8.4767885e-7,0.000065569606,0.0000012884036,0.000076434895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985087,0.000020578986,0.000010786098,0.000046062723,0.000031207754,0.000040481926],"domain_scores_gemma":[0.9979322,0.00038681258,0.00080335693,0.00016304478,0.0002752524,0.0004392752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036480546,0.00013331903,0.00023714367,0.0008742452,0.00032915676,0.00077986345,0.00035448145,0.00028392993,0.0016483339],"category_scores_gemma":[0.0010769694,0.00017055098,0.000114471375,0.00058491435,0.000599124,0.00025890436,0.00042138787,0.00023402939,0.000267752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009490698,0.000030045434,0.9793667,0.000015288168,0.000018140663,0.000059511014,0.0001757396,0.00008618532,0.017960316,0.000113469694,0.000030945306,0.002048877],"study_design_scores_gemma":[0.0000014165278,0.000019842395,0.99926263,0.0000011011433,0.0000029942287,0.00004820091,0.000054640197,0.00007549485,0.00045599986,0.000024595922,0.000052087547,9.838603e-7],"about_ca_topic_score_codex":0.002973104,"about_ca_topic_score_gemma":0.005066787,"teacher_disagreement_score":0.002973104,"about_ca_system_score_codex":0.00023055288,"about_ca_system_score_gemma":0.0001245513,"threshold_uncertainty_score":0.0059115887},"labels":[],"label_agreement":null},{"id":"W2184573973","doi":"10.1088/0004-637x/813/1/73","title":"GONE IN A BLAZE OF GLORY: THE DEMISE OF COMET C/2015 D1 (<i>SOHO</i>)","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Comet; Sublimation (psychology); Light curve; RADIUS; Observatory; Solar System; Debris; Comet dust; Brightness; Formation and evolution of the Solar System","score_opus":0.017484059766536286,"score_gpt":0.24105703732838799,"score_spread":0.2235729775618517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2184573973","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98963004,0.0022250786,0.0003492415,0.0018865274,0.00008310059,0.000008672313,0.00055043155,0.00007495844,0.0051920316],"genre_scores_gemma":[0.9971118,0.0006361071,0.00026709447,0.00050532457,0.00009691499,0.0000025113875,0.0004863709,0.00002463575,0.0008692883],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987483,0.0000140184,0.0000044170674,0.00003130311,0.000037398197,0.000038013808],"domain_scores_gemma":[0.99983144,0.000011461191,0.0000414442,0.000026314085,0.000028417977,0.000060967504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024419485,0.0002041459,0.00020243089,0.00055860693,0.0009488062,0.0010995803,0.0003841529,0.00077884557,0.0010015153],"category_scores_gemma":[0.0005358679,0.00009177737,0.00029174422,0.00036230896,0.00086322246,0.00085096696,0.0008374765,0.0005394953,0.00036584734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013807145,0.00025707396,0.7338206,0.00046906696,0.0003976177,0.025161762,0.018511206,0.0052626007,0.05809023,0.010526486,0.041778073,0.104344696],"study_design_scores_gemma":[0.000022033704,0.0003083927,0.8640782,0.000093102324,0.00012961405,0.008258441,0.006651538,0.0034418805,0.004517909,0.0025907157,0.10983599,0.00007212761],"about_ca_topic_score_codex":0.016879015,"about_ca_topic_score_gemma":0.023462608,"teacher_disagreement_score":0.016879015,"about_ca_system_score_codex":0.0012306478,"about_ca_system_score_gemma":0.00027373445,"threshold_uncertainty_score":0.033561528},"labels":[],"label_agreement":null},{"id":"W2185239949","doi":"10.3847/1538-4357/834/1/53","title":"THE EVOLUTION OF STAR FORMATION ACTIVITY IN CLUSTER GALAXIES OVER 0.15 &lt; z &lt; 1.5","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Star formation; Cluster (spacecraft); Galaxy; Redshift; Galaxy cluster; Population; Astronomy; Stellar mass","score_opus":0.00613133144569153,"score_gpt":0.207915249544692,"score_spread":0.20178391809900048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2185239949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881977,0.000056586734,0.000045657085,0.000026264832,0.0000014021442,0.0000013084698,0.00072615274,0.000012178631,0.00031061596],"genre_scores_gemma":[0.9988481,0.000022145143,0.000053344076,0.000009541218,0.0000024470758,0.0000016955831,0.0008102818,0.000002733615,0.00024969614],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987173,0.000008825227,0.0000058587925,0.000039530358,0.000028646416,0.000045419478],"domain_scores_gemma":[0.9991812,0.00009359807,0.00030082033,0.000046927773,0.00013716955,0.00024017754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030457583,0.00011350875,0.00017589059,0.0011665697,0.00021687405,0.0006201837,0.00024846356,0.0002295275,0.0012415816],"category_scores_gemma":[0.0007389868,0.000083791085,0.00025458544,0.00072523655,0.00025034999,0.00025513605,0.00038044955,0.00021463381,0.0003606638],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045149372,0.000016218159,0.99412364,0.000006305545,0.00003627504,0.000036280995,0.00016052244,0.00048011597,0.0014881592,0.00017706877,0.0004953794,0.0029349278],"study_design_scores_gemma":[7.5772437e-7,0.0000072169437,0.9993755,9.817117e-7,0.000002934485,0.0000128137235,0.000029646468,0.0002733838,0.00009867361,0.000011595914,0.00018512158,0.00000135984],"about_ca_topic_score_codex":0.032460485,"about_ca_topic_score_gemma":0.035880573,"teacher_disagreement_score":0.032460485,"about_ca_system_score_codex":0.00063338614,"about_ca_system_score_gemma":0.00018726368,"threshold_uncertainty_score":0.06454307},"labels":[],"label_agreement":null},{"id":"W2185925527","doi":"10.1088/0004-637x/811/2/100","title":"THE AU MIC DEBRIS DISK: FAR-INFRARED AND SUBMILLIMETER RESOLVED IMAGING","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Planetesimal; Debris disk; James Clerk Maxwell Telescope; Luminosity; Debris; Halo; Bolometer; Thermal emission; Telescope","score_opus":0.01354478800234404,"score_gpt":0.23807919632103405,"score_spread":0.22453440831869,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2185925527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98600626,0.0014537649,0.00085881155,0.000096142896,0.000016448455,0.000017880255,0.0010019403,0.0001554573,0.010393172],"genre_scores_gemma":[0.9958099,0.00032048678,0.0022654356,0.000058093097,0.00003067873,0.000008044966,0.0006809022,0.000016213105,0.0008102878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999918,0.0000044053645,0.0000029116075,0.000024537176,0.000024677485,0.000025587628],"domain_scores_gemma":[0.99987066,0.000014341584,0.000038143728,0.000016337512,0.00002051185,0.000039983774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011584663,0.00015497424,0.00015310098,0.0011164827,0.0002331901,0.00044703687,0.00029104104,0.000283872,0.0011524858],"category_scores_gemma":[0.00023294521,0.00017370158,0.0001288618,0.00062625355,0.000097117445,0.00027356905,0.00034349627,0.0002492204,0.00028190232],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009160294,0.0004043361,0.48356974,0.0004279406,0.00020344253,0.0022504362,0.0008792779,0.0025951813,0.39430544,0.0017938636,0.0056104264,0.10704392],"study_design_scores_gemma":[0.000009015656,0.000052772964,0.9908702,0.000016879225,0.00002788232,0.00083457085,0.00012411924,0.0014550566,0.0032137255,0.00016456416,0.003222262,0.000009074416],"about_ca_topic_score_codex":0.00137277,"about_ca_topic_score_gemma":0.002560615,"teacher_disagreement_score":0.00137277,"about_ca_system_score_codex":0.00020138171,"about_ca_system_score_gemma":0.00007814657,"threshold_uncertainty_score":0.0038554668},"labels":[],"label_agreement":null},{"id":"W2186599455","doi":"10.3847/0004-637x/816/2/95","title":"THE KEPLER-454 SYSTEM: A SMALL, NOT-ROCKY INNER PLANET, A JOVIAN WORLD, AND A DISTANT COMPANION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science Mission Directorate; Smithsonian Astrophysical Observatory; Université de Genève; Danmarks Grundforskningsfond; Science and Technology Facilities Council; National Research Foundation; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; Stellar Astrophysics Centre; Queen's University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; NASA Exoplanet Science Institute; Fundação para a Ciência e a Tecnologia; Harvard University; John Templeton Foundation; W. M. Keck Foundation; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; Planet; Astrophysics; Exoplanet; Astronomy; Radial velocity; Planetary system; RADIUS; Planetary mass; Spectrograph; Stars; Spectral line","score_opus":0.011195683544190933,"score_gpt":0.20257583640417537,"score_spread":0.19138015285998444,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2186599455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99624795,0.00025865674,0.0002935133,0.000035831483,0.0000074204736,0.000008183925,0.00020158103,0.000038298163,0.0029086028],"genre_scores_gemma":[0.99844474,0.00003972879,0.0004961391,0.000016236543,0.00000570659,0.0000020903628,0.00026944946,0.0000036552974,0.00072235125],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998621,0.000015750922,0.000010461483,0.000049551065,0.000031852833,0.000030252977],"domain_scores_gemma":[0.99977964,0.000018405626,0.000076071905,0.000024939292,0.000016014832,0.00008500195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001751739,0.00035604145,0.00021981396,0.00081758917,0.0006977654,0.00082873,0.00025270422,0.00029298654,0.0027344313],"category_scores_gemma":[0.00044144035,0.00019700105,0.00011449854,0.0004460738,0.00029066115,0.0006216431,0.0009262806,0.00027536074,0.0008002132],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007168858,0.00013369828,0.92708385,0.000083287945,0.0000980083,0.0021919252,0.0004346909,0.00058741536,0.038992368,0.0009603601,0.0014370666,0.027280552],"study_design_scores_gemma":[0.000036404927,0.00027553344,0.97026694,0.000018219682,0.000070553746,0.005135543,0.0004360701,0.0021245815,0.007875082,0.00054157194,0.013196237,0.000023248236],"about_ca_topic_score_codex":0.0010609456,"about_ca_topic_score_gemma":0.0014250267,"teacher_disagreement_score":0.0027344313,"about_ca_system_score_codex":0.00027618528,"about_ca_system_score_gemma":0.00015067225,"threshold_uncertainty_score":0.009147584},"labels":[],"label_agreement":null},{"id":"W2187838105","doi":"10.3847/0004-637x/817/2/167","title":"THE JCMT GOULD BELT SURVEY: A FIRST LOOK AT DENSE CORES IN ORION B","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Manitoba; University of Alberta; Université Laval; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; University of Waterloo; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Protostar; Astrophysics; Physics; Molecular cloud; Star formation; Stars; Astronomy","score_opus":0.014328697977873072,"score_gpt":0.23983432474287864,"score_spread":0.22550562676500557,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2187838105","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972938,0.0002265715,0.000048050366,0.00006045362,0.000001547034,0.000008876895,0.0015308994,0.000010383052,0.0008194759],"genre_scores_gemma":[0.99655247,0.00020338352,0.00039830338,0.000067124376,0.000011824236,0.000012222846,0.0022908673,0.00000836895,0.0004554352],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998443,0.000011840215,0.000010186132,0.000041800395,0.000047945054,0.00004400533],"domain_scores_gemma":[0.9993698,0.000053608837,0.00023844665,0.000055258108,0.00007975302,0.00020324746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018244104,0.00016782676,0.00015983982,0.0028472263,0.0005305068,0.00041822362,0.00031503418,0.00024984754,0.0016329001],"category_scores_gemma":[0.0006179788,0.00012546677,0.00012598673,0.00171463,0.00025308493,0.00035694172,0.00088874146,0.0001492929,0.00028026948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022509481,0.000013443562,0.9907981,0.000020394858,0.000012434603,0.00014078962,0.0005162626,0.000018295996,0.0034642685,0.000046680067,0.00050449773,0.004442403],"study_design_scores_gemma":[6.896765e-7,0.0000028155805,0.9992556,0.0000040724635,0.0000015559525,0.000041206826,0.0000960074,0.00001763612,0.0000744469,0.000006053999,0.0004992802,6.946596e-7],"about_ca_topic_score_codex":0.034185622,"about_ca_topic_score_gemma":0.07294996,"teacher_disagreement_score":0.034185622,"about_ca_system_score_codex":0.00040865605,"about_ca_system_score_gemma":0.00023911691,"threshold_uncertainty_score":0.067973256},"labels":[],"label_agreement":null},{"id":"W2188881976","doi":"10.3847/0004-637x/822/2/66","title":"HYPERCALIBRATION: A PAN-STARRS1-BASED RECALIBRATION OF THE SLOAN DIGITAL SKY SURVEY PHOTOMETRY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; National Central University; Deutsche Forschungsgemeinschaft; Durham University; York University; Space Telescope Science Institute; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Goddard Space Flight Center; Harvard University; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University","keywords":"Photometry (optics); Sky; Stars; Photometric system; Apparent magnitude","score_opus":0.014919457073754265,"score_gpt":0.21941711962863808,"score_spread":0.2044976625548838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2188881976","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6781288,0.00081816426,0.21840188,0.0006288647,0.0003564194,0.0005515506,0.025258264,0.051434197,0.02442187],"genre_scores_gemma":[0.7402183,0.0002449666,0.19882919,0.00034701117,0.00009657773,0.0002942387,0.04853764,0.005173246,0.006258801],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9981541,0.00036786258,0.0001446657,0.0006667798,0.000532318,0.00013414117],"domain_scores_gemma":[0.99660206,0.00020844507,0.00037742007,0.0016395537,0.0010899089,0.00008254606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002372299,0.00067931216,0.0006896168,0.0027229697,0.0006885077,0.0015516831,0.0011786922,0.00048407927,0.0053455145],"category_scores_gemma":[0.0048427293,0.00051304704,0.0007920427,0.0027408611,0.0002438182,0.0012076118,0.0015266837,0.00081850117,0.0034998164],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006458029,0.00057777076,0.27898514,0.0003711635,0.00077149685,0.00023980429,0.0015691131,0.07264318,0.050741598,0.0031903333,0.0631637,0.52710086],"study_design_scores_gemma":[0.00020357853,0.00023531912,0.49475822,0.000105381834,0.00030701852,0.0003755046,0.0005093904,0.27447549,0.06350688,0.002851994,0.16245568,0.00021549723],"about_ca_topic_score_codex":0.0144840125,"about_ca_topic_score_gemma":0.02038235,"teacher_disagreement_score":0.0144840125,"about_ca_system_score_codex":0.0010025583,"about_ca_system_score_gemma":0.00081640156,"threshold_uncertainty_score":0.028799415},"labels":[],"label_agreement":null},{"id":"W2189141157","doi":"10.3847/0004-637x/822/2/59","title":"THE BOLOCAM GALACTIC PLANE SURVEY. XIV. PHYSICAL PROPERTIES OF MASSIVE STARLESS AND STAR-FORMING CLUMPS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galactic plane; Astrophysics; Star (game theory); Physics; Star formation; Astronomy; Galaxy","score_opus":0.016807000996186164,"score_gpt":0.23117694453026422,"score_spread":0.21436994353407807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2189141157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93171453,0.0016425101,0.00018268455,0.0001294173,0.000017300987,0.00004101195,0.06276376,0.00012055152,0.0033881587],"genre_scores_gemma":[0.9172548,0.0009993791,0.00056714745,0.00007986364,0.0000490474,0.000048430928,0.07852389,0.000046320027,0.002430936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984825,0.000018360466,0.00001548792,0.00003553273,0.000041457588,0.000040887076],"domain_scores_gemma":[0.9991456,0.00004376581,0.00045521135,0.000066195345,0.00009614546,0.0001930412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030143428,0.00027073896,0.00027794298,0.0034897383,0.00022286574,0.0006110173,0.0002936633,0.00015287762,0.0033307092],"category_scores_gemma":[0.00067863043,0.00014605741,0.00023687408,0.0026569623,0.0001253099,0.00019745783,0.00047844934,0.00018721832,0.0017251907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000064038024,0.000011293491,0.9911295,0.00002635816,0.000028256693,0.00003022808,0.00006829071,0.00004248046,0.00074789114,0.000041873187,0.0033942766,0.004415551],"study_design_scores_gemma":[0.0000049870055,0.00000628549,0.9989054,0.000007374627,0.000004847915,0.000024341549,0.00003809386,0.000037060083,0.000061653496,0.0000072395374,0.00090182264,9.738588e-7],"about_ca_topic_score_codex":0.03768848,"about_ca_topic_score_gemma":0.047902748,"teacher_disagreement_score":0.03768848,"about_ca_system_score_codex":0.00042005331,"about_ca_system_score_gemma":0.0002140579,"threshold_uncertainty_score":0.07493824},"labels":[],"label_agreement":null},{"id":"W2189810354","doi":"10.1088/0004-637x/812/2/138","title":"EVIDENCE FOR THE UNIVERSALITY OF PROPERTIES OF RED-SEQUENCE GALAXIES IN X-RAY- AND RED-SEQUENCE-SELECTED CLUSTERS AT<i>z</i>∼ 1","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Centro de Astrofísica y Tecnologías Afines; California Institute of Technology","keywords":"Galaxy cluster; Cluster (spacecraft); Galaxy; Galaxy groups and clusters; Stars; Universality (dynamical systems); Galaxy group","score_opus":0.061953408080343345,"score_gpt":0.25785419965378714,"score_spread":0.1959007915734438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2189810354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99465334,0.000317033,0.00045848824,0.00012858785,0.000007198224,0.000006407364,0.00034732287,0.000073712414,0.0040078308],"genre_scores_gemma":[0.9992285,0.000040369196,0.000110343826,0.000036528556,0.0000055667083,0.000002836964,0.00024045062,0.000009658274,0.00032584014],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959475,0.000034082743,0.00002204681,0.00019905453,0.000063782936,0.00008634228],"domain_scores_gemma":[0.99565315,0.0007381867,0.0011971697,0.0009171689,0.00069499,0.0007993779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055768073,0.00014764068,0.0003054223,0.0023277756,0.00077738485,0.0012042021,0.0006582535,0.00049540255,0.0064072744],"category_scores_gemma":[0.002804484,0.00028709866,0.00022881321,0.0014432535,0.0013383739,0.000696016,0.0011830678,0.00042799622,0.0007960454],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011290309,0.0000301231,0.9853297,0.00002571229,0.00005005503,0.000034446046,0.0005823491,0.00006675375,0.007167601,0.00081461004,0.0003146584,0.005471073],"study_design_scores_gemma":[0.0000020527054,0.000008611747,0.9991943,0.0000021867802,0.00000617511,0.00004414623,0.00013880934,0.000062272615,0.0001606414,0.00017455363,0.00020404525,0.0000021767719],"about_ca_topic_score_codex":0.00905838,"about_ca_topic_score_gemma":0.0128997695,"teacher_disagreement_score":0.00905838,"about_ca_system_score_codex":0.0004889761,"about_ca_system_score_gemma":0.00039282982,"threshold_uncertainty_score":0.021434426},"labels":[],"label_agreement":null},{"id":"W2190402949","doi":"10.3847/0004-637x/832/1/92","title":"MEASURING NEUTRON STAR RADII VIA PULSE PROFILE MODELING WITH NICER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Physics; Pulsar; Astrophysics; Payload (computing); Equation of state; Pulse (music); Computational physics; Computer science; Optics","score_opus":0.021286739192318913,"score_gpt":0.27555263921150275,"score_spread":0.2542659000191838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2190402949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.63106614,0.00018851852,0.3582197,0.00021777913,0.000024441017,0.000064952415,0.0007390666,0.0031758198,0.00630356],"genre_scores_gemma":[0.9568407,0.000073724994,0.04191987,0.00003103966,0.000007760663,0.000026816004,0.0004168723,0.00013215347,0.0005510537],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99971575,0.00009177895,0.000016838727,0.0000679107,0.000083024024,0.000024675272],"domain_scores_gemma":[0.99877554,0.00052043644,0.00024048562,0.00024945856,0.00015216554,0.00006188705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009633073,0.00046335338,0.00045563895,0.0007046091,0.00027119106,0.00065191346,0.0008934146,0.0006706074,0.0007099667],"category_scores_gemma":[0.0029540353,0.00038181353,0.00053400506,0.00047525528,0.00028091393,0.00080770755,0.0005031809,0.00046051832,0.00039238256],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033587747,0.00010571666,0.028489994,0.000060746945,0.000076175726,0.00011164957,0.00013737023,0.92263585,0.019262228,0.004294351,0.00040285275,0.02408713],"study_design_scores_gemma":[0.0000070882907,0.000019223831,0.0018807987,0.0000025991703,0.0000063821485,0.000026920456,0.0000043858972,0.99339384,0.0038572734,0.0005410349,0.0002490786,0.000011321171],"about_ca_topic_score_codex":0.0040521706,"about_ca_topic_score_gemma":0.0029533063,"teacher_disagreement_score":0.0040521706,"about_ca_system_score_codex":0.0007941244,"about_ca_system_score_gemma":0.00037814965,"threshold_uncertainty_score":0.008057177},"labels":[],"label_agreement":null},{"id":"W2190919103","doi":"10.1088/0004-637x/814/2/163","title":"IMPLICATIONS FOR THE FORMATION OF BLUE STRAGGLER STARS FROM<i>HST</i>ULTRAVIOLET OBSERVATIONS OF NGC 188","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Blue straggler; Photometry (optics); Stars; White dwarf; Roche lobe; Star cluster; Globular cluster; Star formation; Hertzsprung–Russell diagram; Hubble space telescope","score_opus":0.04820459622426615,"score_gpt":0.26230653356043776,"score_spread":0.2141019373361716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2190919103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99875677,0.000054014698,0.00009176072,0.000030237985,0.0000019982397,0.000001926643,0.00018438113,0.000013620595,0.0008652863],"genre_scores_gemma":[0.9995915,0.00003197318,0.00007494944,0.000010705181,0.000002925057,0.0000012353373,0.000160621,0.0000022228842,0.0001237775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999143,0.000008176653,0.0000069616945,0.000025468851,0.00002170559,0.000023436794],"domain_scores_gemma":[0.99926597,0.00009363324,0.0003687461,0.00005148157,0.000051649655,0.0001684362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017136357,0.00021134382,0.0001498734,0.00057343947,0.00037507512,0.00054648274,0.0002525486,0.00022348453,0.0025879545],"category_scores_gemma":[0.0006578038,0.00010625151,0.0001305621,0.00035515308,0.0003730235,0.00026409555,0.00030243633,0.00017791588,0.00036405952],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010125081,0.00001611149,0.9841346,0.000020034578,0.000008866235,0.00024621657,0.00018364671,0.00035265618,0.012398774,0.00017056127,0.00016628466,0.0022010102],"study_design_scores_gemma":[0.0000026614637,0.000025714622,0.99758756,0.000004930554,0.0000061992514,0.00021004655,0.00018422432,0.00041797291,0.0010836358,0.000085270905,0.00038973146,0.000002091008],"about_ca_topic_score_codex":0.0061676037,"about_ca_topic_score_gemma":0.011104961,"teacher_disagreement_score":0.0061676037,"about_ca_system_score_codex":0.00036579728,"about_ca_system_score_gemma":0.00014785849,"threshold_uncertainty_score":0.012263358},"labels":[],"label_agreement":null},{"id":"W2191420841","doi":"10.3847/0004-637x/820/1/45","title":"MODELING GD-1 GAPS IN A MILKY WAY POTENTIAL","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Halo; Milky Way; Physics; Astrophysics; Dark matter; Computational physics; Stars; Galaxy","score_opus":0.007085236666038723,"score_gpt":0.20608036750145758,"score_spread":0.19899513083541887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2191420841","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974648,0.00002783401,0.00066966354,0.00008773822,0.0000043174814,0.0000079696965,0.00011643739,0.000032045697,0.0015892733],"genre_scores_gemma":[0.9988894,0.0000135901455,0.00054212724,0.000019795338,0.0000025044076,0.0000071899926,0.0001400379,0.000013667924,0.00037160216],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999136,0.000019492929,0.0000026790017,0.000014252318,0.000015097974,0.00003489789],"domain_scores_gemma":[0.99942756,0.00019622777,0.00007344485,0.000039478367,0.00008264662,0.00018069232],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038843087,0.00025550582,0.00039264318,0.00055723067,0.0006248456,0.0007218248,0.0008648917,0.0008234571,0.001301235],"category_scores_gemma":[0.0023292822,0.0002124676,0.00047533656,0.00041578957,0.0006686609,0.00054525945,0.00083483366,0.00045559573,0.00015029286],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014437466,0.0000783369,0.025224835,0.000020160567,0.000038091075,0.0002974759,0.00012313634,0.96634156,0.0010764645,0.004759859,0.0006164737,0.0012792223],"study_design_scores_gemma":[0.000060199127,0.00005362474,0.004621384,0.0000056912636,0.000008384473,0.000026319398,0.000082299164,0.9933541,0.00026261146,0.001210035,0.00030699812,0.000008244201],"about_ca_topic_score_codex":0.038609914,"about_ca_topic_score_gemma":0.019198243,"teacher_disagreement_score":0.038609914,"about_ca_system_score_codex":0.0018379505,"about_ca_system_score_gemma":0.00090095174,"threshold_uncertainty_score":0.076770365},"labels":[],"label_agreement":null},{"id":"W2191540195","doi":"10.1088/0004-637x/811/2/111","title":"DEEP<i>CHANDRA</i>,<i>HST</i>-COS, AND MEGACAM OBSERVATIONS OF THE PHOENIX CLUSTER: EXTREME STAR FORMATION AND AGN FEEDBACK ON HUNDRED KILOPARSEC SCALES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Fonds de recherche du Québec – Nature et technologies; Space Telescope Science Institute; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Intracluster medium; Star formation; Galaxy; Astronomy; Active galactic nucleus; Stars; Population; Quasar; Redshift; Galaxy cluster","score_opus":0.025805886173123044,"score_gpt":0.21203749698583355,"score_spread":0.1862316108127105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2191540195","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99553126,0.00007523324,0.00039795082,0.00005506713,0.000003622219,0.000008763535,0.0014585688,0.00008586074,0.0023835644],"genre_scores_gemma":[0.99397635,0.00013966497,0.0022139219,0.00005820237,0.00002459222,0.00000764001,0.0027515898,0.000021061014,0.00080690713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999554,0.0000018427244,0.0000015237247,0.00001606714,0.000012305027,0.000012874667],"domain_scores_gemma":[0.99981445,0.000012225441,0.00005874758,0.000022741608,0.000015082677,0.00007672321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010966042,0.00024636812,0.000119671815,0.00061557983,0.0002487513,0.00043365525,0.0003506107,0.0001378368,0.0017847735],"category_scores_gemma":[0.00017271577,0.00016448883,0.00012705223,0.00039793245,0.00016454577,0.00028615835,0.0004387874,0.0003706003,0.00023086766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004180027,0.00019431922,0.7879487,0.0000980255,0.00018403707,0.0013530351,0.0004190384,0.0025650177,0.17426139,0.00065307907,0.004204499,0.0277008],"study_design_scores_gemma":[0.000017432018,0.000045511686,0.99021775,0.0000068807253,0.000025099758,0.0004705846,0.0000697054,0.0014967354,0.0051489333,0.00014762869,0.0023462847,0.000007536925],"about_ca_topic_score_codex":0.0048727836,"about_ca_topic_score_gemma":0.012868719,"teacher_disagreement_score":0.0048727836,"about_ca_system_score_codex":0.00022697108,"about_ca_system_score_gemma":0.00012466227,"threshold_uncertainty_score":0.009688795},"labels":[],"label_agreement":null},{"id":"W2191829672","doi":"10.3847/0004-637x/819/2/156","title":"MULTIWAVELENGTH STUDY OF QUIESCENT STATES OF Mrk 421 WITH UNPRECEDENTED HARD X-RAY COVERAGE PROVIDED BY NuSTAR IN 2013","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Japan Society for the Promotion of Science; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Istituto Nazionale di Fisica Nucleare; Natural Sciences and Engineering Research Council of Canada; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Bilim Akademisi; Smithsonian Institution; U.S. Department of Energy; Vetenskapsrådet; Max-Planck-Gesellschaft; National Research Foundation; High Energy Accelerator Research Organization; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Hrvatska Zaklada za Znanost; European Regional Development Fund; Bundesministerium für Bildung und Forschung; Russian Foundation for Basic Research; NASA Headquarters; Office of Science; Academy of Finland; Deutsche Forschungsgemeinschaft; Centre National d’Etudes Spatiales; SLAC National Accelerator Laboratory; Ministry of Education, Culture, Sports, Science and Technology; California Institute of Technology; Shota Rustaveli National Science Foundation; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; Türkiye Bilimsel ve Teknolojik Araştırma Kurumu; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Agenzia Spaziale Italiana; National Science Foundation","keywords":"Physics; Astrophysics; X-ray; Astronomy; Optics","score_opus":0.005716281213189412,"score_gpt":0.20924580897839729,"score_spread":0.20352952776520788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2191829672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977182,0.00024617385,0.0002774419,0.000028676322,0.0000048910524,0.000003667563,0.0004767192,0.000053104963,0.0011911629],"genre_scores_gemma":[0.9969501,0.00009771796,0.00042654044,0.000022400727,0.0000145438,0.0000052084265,0.002054363,0.000032431606,0.00039681027],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998142,0.000011117957,0.000008775506,0.000065048225,0.00005896484,0.00004177208],"domain_scores_gemma":[0.9996257,0.000020285666,0.00015165549,0.000051621362,0.00007306291,0.00007765604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030338182,0.00023385651,0.00040934145,0.0012331587,0.00048290935,0.0007906258,0.00029728937,0.00021159808,0.0005694347],"category_scores_gemma":[0.0004003076,0.00021927578,0.000279626,0.00094399025,0.00024000564,0.00024539663,0.0007327547,0.0003121173,0.0003913191],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082525564,0.00013728629,0.77237546,0.0001621967,0.00029579384,0.0015537721,0.0018464561,0.0015844207,0.18891999,0.0005326371,0.0018258166,0.029940834],"study_design_scores_gemma":[0.0000039645033,0.00003887977,0.9948488,0.00000527169,0.000021970236,0.0002852618,0.00014754206,0.00055834185,0.0021336605,0.000052327534,0.0018959199,0.000008105516],"about_ca_topic_score_codex":0.0031630835,"about_ca_topic_score_gemma":0.005932073,"teacher_disagreement_score":0.0031630835,"about_ca_system_score_codex":0.0003320185,"about_ca_system_score_gemma":0.00017423056,"threshold_uncertainty_score":0.0062893033},"labels":[],"label_agreement":null},{"id":"W2192486162","doi":"10.1086/378886","title":"Raman‐scattered He<scp>ii</scp>λ6545 Line in the Symbiotic Star V1016 Cygni","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Symbiotic star; Raman scattering; Scattering; Emission spectrum; Line (geometry); Radiation; Binary number; Flux (metallurgy); Photon","score_opus":0.01201177226729151,"score_gpt":0.23426478721914554,"score_spread":0.22225301495185404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2192486162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987501,0.00005414017,0.00022967403,0.000023177943,0.0000018387225,0.0000015855738,0.000050495,0.000019326671,0.00086969486],"genre_scores_gemma":[0.9994272,0.000022169863,0.0001990764,0.000015477071,0.0000023651435,0.0000024121994,0.0001003664,0.000005388001,0.00022561841],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995446,0.0000030199515,0.000001240412,0.000015585973,0.000012776681,0.000012958851],"domain_scores_gemma":[0.9999161,0.000012140865,0.000022517157,0.0000073002534,0.000010801892,0.000031124066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000096680385,0.00025024734,0.00016228377,0.00034986978,0.00030383278,0.00029061156,0.00025986464,0.0002791199,0.00080421235],"category_scores_gemma":[0.00015409938,0.00012729915,0.00013562059,0.00026601003,0.00021575348,0.00010503821,0.00023968368,0.00019881522,0.0002381597],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003307253,0.000085894986,0.15543078,0.000053387754,0.000062206964,0.0018177711,0.00034452195,0.002215335,0.8291476,0.0006521802,0.0004097301,0.00944986],"study_design_scores_gemma":[0.000025078596,0.00011445254,0.94588804,0.000010906613,0.000027360033,0.0006251237,0.00021923907,0.008449409,0.043494653,0.0003191988,0.00081269577,0.000013978336],"about_ca_topic_score_codex":0.0037403656,"about_ca_topic_score_gemma":0.0038575782,"teacher_disagreement_score":0.0037403656,"about_ca_system_score_codex":0.0004337092,"about_ca_system_score_gemma":0.000104824285,"threshold_uncertainty_score":0.0074371696},"labels":[],"label_agreement":null},{"id":"W2193383097","doi":"10.1088/0004-637x/814/1/22","title":"DETECTION OF INFALL IN THE PROTOSTAR B335 WITH ALMA","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Astronomical Observatory of Japan; National Research Foundation of Korea; Ministry of Science, ICT and Future Planning; National Science Council; National Research Foundation; University of Texas at Austin; National Radio Astronomy Observatory; National Institutes of Natural Sciences; H. Lundbeck A/S; Korea Astronomy and Space Science Institute; Lundbeckfonden; National Science Foundation","keywords":"Physics; Protostar; Astrophysics; Opacity; Solar mass; RADIUS; Redshift; Astronomy; Solar radius; Star formation; Luminosity; Stellar mass; Stars; Plasma; Coronal mass ejection; Optics; Solar wind; Galaxy","score_opus":0.013943349935695367,"score_gpt":0.23501258713506032,"score_spread":0.22106923719936494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2193383097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99306935,0.00049686525,0.00039185505,0.0001871167,0.000027656046,0.0000151284,0.00047334994,0.00009082582,0.0052476274],"genre_scores_gemma":[0.9977785,0.00008219015,0.0007398581,0.00010474193,0.000017315222,0.0000068846894,0.0005220927,0.0000108492595,0.00073741615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999808,0.000016234728,0.000008297979,0.00007771933,0.000046621793,0.00004307483],"domain_scores_gemma":[0.99949765,0.000051728483,0.00015621007,0.000056723835,0.000087427994,0.00015023923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034508095,0.00021630427,0.00014542678,0.0011772156,0.00081700546,0.0005672816,0.00027633435,0.0005641731,0.0020636888],"category_scores_gemma":[0.000583353,0.00020953239,0.00023813223,0.00077216467,0.00032582702,0.00035055456,0.00069863873,0.00032841234,0.000419325],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061649986,0.00008861377,0.7969376,0.00008726724,0.00009528382,0.0014426414,0.00065125915,0.00014754891,0.17958793,0.00072563085,0.0017569567,0.017862711],"study_design_scores_gemma":[0.00001136158,0.000089956346,0.98886067,0.000019260147,0.000039633884,0.00075682206,0.00038451276,0.00052818016,0.004427378,0.00018664291,0.0046859127,0.000009605937],"about_ca_topic_score_codex":0.008174437,"about_ca_topic_score_gemma":0.014719158,"teacher_disagreement_score":0.008174437,"about_ca_system_score_codex":0.0004605001,"about_ca_system_score_gemma":0.00023716809,"threshold_uncertainty_score":0.01625371},"labels":[],"label_agreement":null},{"id":"W2194030965","doi":"10.3847/0004-637x/817/2/95","title":"EXPLORING X-RAY BINARY POPULATIONS IN COMPACT GROUP GALAXIES WITH CHANDRA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Galaxy; Active galactic nucleus; Luminosity; Spiral galaxy; Elliptical galaxy; Binary number; Luminous infrared galaxy; Galaxy formation and evolution; Cosmology","score_opus":0.04367011282141683,"score_gpt":0.23693161636201202,"score_spread":0.19326150354059518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2194030965","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993383,0.00009796242,0.00025047234,0.0000065346935,8.6315515e-7,0.0000038174007,0.00010411013,0.000014246456,0.00018364468],"genre_scores_gemma":[0.9992545,0.000035272762,0.00046806625,0.0000044211565,0.0000030915432,0.0000036993945,0.00017806467,0.0000045748607,0.000048213435],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99944216,0.00012071022,0.00003820079,0.00015975835,0.00011420431,0.00012486367],"domain_scores_gemma":[0.9967788,0.00087768905,0.0011389711,0.0004489366,0.00022585514,0.000529829],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001372121,0.0003821968,0.0006421932,0.004577189,0.0004666957,0.0011338341,0.000535501,0.00028362067,0.0011090471],"category_scores_gemma":[0.002797167,0.0003393359,0.00050686876,0.0021305953,0.0005155027,0.0007154557,0.0013681817,0.00029484465,0.00023957812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013492593,0.000038196507,0.98983556,0.00002465338,0.00013155286,0.000075933414,0.00036393284,0.00046047757,0.0038185474,0.0001680725,0.0000653847,0.004882725],"study_design_scores_gemma":[0.000008181116,0.00005802262,0.997051,0.000008275286,0.000035707788,0.00016159148,0.00019729693,0.0014435764,0.00067157537,0.00012871137,0.00022799616,0.000008026069],"about_ca_topic_score_codex":0.004814939,"about_ca_topic_score_gemma":0.0053607887,"teacher_disagreement_score":0.004814939,"about_ca_system_score_codex":0.00031547208,"about_ca_system_score_gemma":0.00019080861,"threshold_uncertainty_score":0.009573877},"labels":[],"label_agreement":null},{"id":"W2194080530","doi":"10.1086/422091","title":"The<i>Swift</i>Gamma‐Ray Burst Mission","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":4209,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Gamma-ray burst; Physics; Afterglow; Redshift; Astrophysics; Astronomy; Observatory; Swift; Telescope; Field of view; Spacecraft; Galaxy; Optics","score_opus":0.009517234401800693,"score_gpt":0.2310574094504192,"score_spread":0.2215401750486185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2194080530","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.28072336,0.0050024004,0.045078862,0.01128445,0.0035567617,0.0017120809,0.21156149,0.022065144,0.4190155],"genre_scores_gemma":[0.36519998,0.003003698,0.12941961,0.0047117015,0.0018809116,0.0012838837,0.41745517,0.002604915,0.0744401],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9996088,0.000033392644,0.000017158334,0.000072181436,0.00017440817,0.00009400462],"domain_scores_gemma":[0.9991861,0.000038751972,0.00019055934,0.0001262191,0.00023740657,0.0002209606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014795448,0.0007343038,0.00050972996,0.0010278911,0.0011617745,0.0015702411,0.0008721087,0.00050069724,0.0060291514],"category_scores_gemma":[0.00092933537,0.0002490128,0.00037563924,0.00077281875,0.00032554197,0.0010001198,0.0016860733,0.0011044514,0.0032668079],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087142235,0.0003080574,0.06256692,0.00031876966,0.00017252378,0.00035763308,0.00036595738,0.0018127654,0.03053244,0.010579592,0.62219554,0.26991838],"study_design_scores_gemma":[0.00037483228,0.00039753297,0.14594422,0.00014282664,0.00009897181,0.00028996592,0.00018048471,0.00848948,0.012143409,0.006359958,0.8254877,0.00009068749],"about_ca_topic_score_codex":0.009754851,"about_ca_topic_score_gemma":0.011831531,"teacher_disagreement_score":0.009754851,"about_ca_system_score_codex":0.000665761,"about_ca_system_score_gemma":0.0017595927,"threshold_uncertainty_score":0.020169556},"labels":[],"label_agreement":null},{"id":"W2194676804","doi":"10.3847/0004-637x/824/2/82","title":"UNCERTAINTIES IN GALACTIC CHEMICAL EVOLUTION MODELS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Fonds de recherche du Québec – Nature et technologies; Los Alamos National Laboratory; Natural Sciences and Engineering Research Council of Canada; Canarie; Canadian Foundation for AIDS Research; Alexander von Humboldt-Stiftung; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; U.S. Department of Energy; National Science Foundation","keywords":"Milky Way; Metallicity; Supernova; Physics; Astrophysics; Galaxy; Monte Carlo method; Initial mass function; Range (aeronautics); Function (biology); Statistical physics; Statistics; Mathematics; Star formation","score_opus":0.012501114382090164,"score_gpt":0.2174756260892411,"score_spread":0.20497451170715092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2194676804","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8513705,0.000504068,0.12814344,0.0004809151,0.00004278877,0.00012768449,0.0012683499,0.00038439245,0.017677702],"genre_scores_gemma":[0.99172485,0.0001474664,0.006230573,0.00004779253,0.000011519528,0.000051063336,0.0003821764,0.000048461756,0.0013561897],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99876463,0.000537882,0.000061598075,0.00027416574,0.00024844275,0.00011329643],"domain_scores_gemma":[0.996469,0.0022863704,0.00039590077,0.00032925725,0.00041156137,0.000107852626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023265493,0.0009241482,0.000884796,0.0012647604,0.00069412094,0.0024412132,0.0022809673,0.0012486224,0.002687928],"category_scores_gemma":[0.009226738,0.0005163685,0.001113882,0.0009831833,0.0010488944,0.0015969343,0.0011477679,0.00081523735,0.0004227077],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000212584,0.000011258232,0.004240124,0.000011241131,0.000027773658,0.000041460175,0.00002843956,0.9877977,0.00020617903,0.0065852446,0.000069801936,0.0009595373],"study_design_scores_gemma":[0.000016214195,0.000020448964,0.0015025714,0.000011631352,0.000018497602,0.000030218298,0.000024466062,0.98971796,0.00036438185,0.007766966,0.0005108689,0.000015885958],"about_ca_topic_score_codex":0.01558263,"about_ca_topic_score_gemma":0.0053816494,"teacher_disagreement_score":0.01558263,"about_ca_system_score_codex":0.0021986763,"about_ca_system_score_gemma":0.0007762622,"threshold_uncertainty_score":0.030983865},"labels":[],"label_agreement":null},{"id":"W2196436033","doi":"10.3847/0004-637x/820/1/39","title":"SECURE MASS MEASUREMENTS FROM TRANSIT TIMING: 10 KEPLER EXOPLANETS BETWEEN 3 AND 8 M <sub>⊕</sub> WITH DIVERSE DENSITIES AND INCIDENT FLUXES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":144,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Université de Montréal","funders":"","keywords":"Exoplanet; Transit (satellite); Planet; RADIUS; Orbit (dynamics); Range (aeronautics); Planetary system; Orbital decay; Apsidal precession","score_opus":0.023046917446424238,"score_gpt":0.2063669909554638,"score_spread":0.18332007350903956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2196436033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990125,0.000015468984,0.00034442544,0.0000022670106,8.341799e-7,0.0000031710808,0.0002833385,0.000013105601,0.00032488917],"genre_scores_gemma":[0.9984341,0.0000099524395,0.000618992,0.0000017616507,0.0000018154908,0.0000031950706,0.0008183032,0.0000044831654,0.000107342734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997662,0.000029623172,0.000028141827,0.00009692652,0.000042060477,0.000037112084],"domain_scores_gemma":[0.99874485,0.00032343654,0.00040899235,0.00023436516,0.0001494243,0.00013896883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035089056,0.00031077134,0.00024243523,0.0011983704,0.00037064834,0.00047078848,0.00026492827,0.00023107354,0.0011494303],"category_scores_gemma":[0.0017971429,0.00019456753,0.00023080847,0.00082181883,0.00021675786,0.0004629446,0.000640367,0.0002369746,0.00049193774],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000333924,0.000034823162,0.97477055,0.00001460488,0.000054235672,0.000094133255,0.00017836642,0.0011882735,0.0124632595,0.000114941264,0.00008084214,0.010672028],"study_design_scores_gemma":[0.000013295183,0.0001748538,0.98158425,0.0000060846623,0.00004638099,0.0003254755,0.0002818739,0.0064196866,0.009942322,0.00019039631,0.0010029589,0.000012431002],"about_ca_topic_score_codex":0.0013340522,"about_ca_topic_score_gemma":0.0022572028,"teacher_disagreement_score":0.0013340522,"about_ca_system_score_codex":0.00022032112,"about_ca_system_score_gemma":0.00012468724,"threshold_uncertainty_score":0.0038451552},"labels":[],"label_agreement":null},{"id":"W2200250972","doi":"10.1088/0004-637x/805/2/115","title":"VARIABLE PROTOSTELLAR ACCRETION WITH EPISODIC BURSTS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":208,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Gravitational instability; Accretion (finance); Angular momentum; Gravitation; Accretion disc; Instability; Luminosity; Protostar","score_opus":0.014086528901134453,"score_gpt":0.23325529275706827,"score_spread":0.2191687638559338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2200250972","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9795216,0.00035821187,0.01739534,0.000066239685,0.000020822421,0.000023063558,0.00021939662,0.00014974455,0.002245697],"genre_scores_gemma":[0.9978765,0.000063178995,0.001552707,0.000009239613,0.000010446176,0.000012303217,0.00010028276,0.000014672624,0.00036059145],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99992263,0.000015169654,0.0000052547257,0.000018702249,0.000014927692,0.000023334222],"domain_scores_gemma":[0.99978405,0.000055446057,0.000071733724,0.000030579162,0.00001972288,0.000038467984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013728588,0.00041808884,0.00027589526,0.00031234292,0.00024377635,0.000527751,0.00081383955,0.0006008954,0.0008426431],"category_scores_gemma":[0.0007832115,0.00013996828,0.0004672904,0.00042059083,0.00030460517,0.00034744054,0.00045175225,0.00028471358,0.00010873172],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000104212864,0.000060215094,0.06312567,0.000043454984,0.000064254644,0.000641945,0.00009497072,0.92120636,0.003919387,0.0054186815,0.00035316474,0.004967682],"study_design_scores_gemma":[0.000022472286,0.000026892061,0.012094824,0.0000056407002,0.000015955218,0.00012232037,0.000021843665,0.9846771,0.0008816028,0.0015452314,0.00057954225,0.0000065104055],"about_ca_topic_score_codex":0.0057816687,"about_ca_topic_score_gemma":0.0019946375,"teacher_disagreement_score":0.0057816687,"about_ca_system_score_codex":0.00045242388,"about_ca_system_score_gemma":0.00025135855,"threshold_uncertainty_score":0.011496067},"labels":[],"label_agreement":null},{"id":"W2200704433","doi":"10.1086/505290","title":"Deceleration of a Relativistic, Photon‐rich Shell: End of Preacceleration, Damping of Magnetohydrodynamic Turbulence, and the Emission Mechanism of Gamma‐Ray Bursts","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Gamma-ray burst; Lorentz factor; Magnetic field; Compton scattering; Photon; Magnetohydrodynamics; Computational physics; Classical mechanics; Optics; Quantum mechanics","score_opus":0.005555896270844131,"score_gpt":0.20507544861706425,"score_spread":0.19951955234622012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2200704433","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98672175,0.0003583043,0.00658802,0.0001255908,0.000013670996,0.000010580128,0.000023304701,0.00008692611,0.006071915],"genre_scores_gemma":[0.998353,0.00007579684,0.0004639222,0.000009998673,0.000010212949,0.000005462418,0.000010730877,0.000019092531,0.0010517801],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996626,0.000005420209,0.0000014796774,0.000006853845,0.0000063082075,0.000013747127],"domain_scores_gemma":[0.99991167,0.00001640829,0.000029215424,0.000008768005,0.00000765482,0.000026296628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010751871,0.00033400464,0.0001546983,0.00018117453,0.0002671999,0.00082716,0.00034453592,0.00031304173,0.00092622114],"category_scores_gemma":[0.00035032604,0.00014413241,0.00025286232,0.00007769139,0.0004541239,0.0003568276,0.0005168491,0.0003129477,0.00013295887],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001744866,0.00032938027,0.10119328,0.00027731032,0.00014624304,0.008540915,0.0024992288,0.21073072,0.3802719,0.25390494,0.0018796927,0.038481638],"study_design_scores_gemma":[0.00021287282,0.00076186535,0.29115948,0.00006905757,0.000060294296,0.0021492383,0.00058680074,0.6106004,0.03062263,0.058956243,0.0047068526,0.000114234965],"about_ca_topic_score_codex":0.00099838,"about_ca_topic_score_gemma":0.00038170777,"teacher_disagreement_score":0.00099838,"about_ca_system_score_codex":0.00034495347,"about_ca_system_score_gemma":0.000102551065,"threshold_uncertainty_score":0.0030985475},"labels":[],"label_agreement":null},{"id":"W2201155275","doi":"10.1088/0004-637x/812/2/151","title":"DYNAMICS OF SELF-GRAVITY WAKES IN DENSE PLANETARY RINGS. I. PITCH ANGLE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Fluid dynamics and aerodynamics studies","field":"Engineering","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Pitch angle; Autocorrelation; Dynamics (music); Viewing angle; Spiral (railway); Surface (topology)","score_opus":0.006551261185036986,"score_gpt":0.18958930305817304,"score_spread":0.18303804187313605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2201155275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99342865,0.000091558286,0.004882424,0.000044619475,0.000013545439,0.000011332305,0.000038342285,0.000054132743,0.0014354547],"genre_scores_gemma":[0.9989323,0.000027424954,0.0008019177,0.000008912024,0.000003838468,0.0000042013835,0.000032794775,0.000009502555,0.00017905638],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999387,0.000007880073,0.0000034413674,0.0000095124915,0.000014219332,0.000026184876],"domain_scores_gemma":[0.9997011,0.00006661108,0.000086207714,0.000036241865,0.000037498186,0.000072349234],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001594562,0.0002391543,0.0002888886,0.0003511223,0.0003692306,0.00032732863,0.00034086354,0.0003667439,0.0006509459],"category_scores_gemma":[0.0007539163,0.00021405566,0.00039290005,0.0001655083,0.0006468241,0.00062877923,0.00056580687,0.00032923243,0.000079530684],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035016856,0.00020714712,0.04892929,0.00009719176,0.00011093667,0.0009897725,0.00048251761,0.8802873,0.053741153,0.0061525665,0.00056186796,0.008090115],"study_design_scores_gemma":[0.000040361298,0.0000918757,0.01559768,0.000007695864,0.000012728293,0.00010342825,0.00008962329,0.9790795,0.0033843112,0.001299141,0.0002735535,0.000020157251],"about_ca_topic_score_codex":0.0026137324,"about_ca_topic_score_gemma":0.0011766276,"teacher_disagreement_score":0.0026137324,"about_ca_system_score_codex":0.00027665493,"about_ca_system_score_gemma":0.0002679221,"threshold_uncertainty_score":0.005197048},"labels":[],"label_agreement":null},{"id":"W2202894114","doi":"10.3847/0004-637x/818/2/130","title":"ON GALACTIC DENSITY MODELING IN THE PRESENCE OF DUST EXTINCTION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":266,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Extinction (optical mineralogy); Physics; Stars; Astrophysics; Sky; Galaxy; Astronomy; Optics","score_opus":0.020808696765288355,"score_gpt":0.2328044039883342,"score_spread":0.21199570722304587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2202894114","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.65101725,0.0006203621,0.33787248,0.0007645955,0.00006098983,0.0000706853,0.00042071426,0.00044485446,0.008728053],"genre_scores_gemma":[0.9873603,0.00018599043,0.0102991015,0.00006189688,0.000042473806,0.00003292624,0.00011274039,0.00008277427,0.0018218113],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996747,0.00014980738,0.000014140238,0.000061550345,0.00005056725,0.00004924234],"domain_scores_gemma":[0.99838364,0.0009942015,0.00021933341,0.000087921275,0.00021519576,0.000099726625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013484001,0.00064742414,0.0005028146,0.0009956388,0.00049652864,0.0011415804,0.0016327827,0.00093248,0.00091744977],"category_scores_gemma":[0.005762213,0.00043158708,0.00066647393,0.0005517948,0.0008100317,0.0010624075,0.00069491484,0.00051005784,0.00021889289],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000019562187,0.000015213051,0.008342077,0.000009735989,0.000020426756,0.0000999205,0.000054200704,0.9773366,0.0004109681,0.0114127165,0.00020739838,0.0020712619],"study_design_scores_gemma":[0.0000020594591,0.0000021224798,0.0005196755,0.0000016556269,0.0000033305807,0.000009060419,0.0000056507342,0.9983668,0.000049857594,0.00094777136,0.000089619396,0.000002476258],"about_ca_topic_score_codex":0.046603277,"about_ca_topic_score_gemma":0.015434251,"teacher_disagreement_score":0.046603277,"about_ca_system_score_codex":0.0015417689,"about_ca_system_score_gemma":0.0005729768,"threshold_uncertainty_score":0.092664},"labels":[],"label_agreement":null},{"id":"W2203175835","doi":"10.3847/0004-637x/823/1/30","title":"THE STELLAR POPULATION STRUCTURE OF THE GALACTIC DISK","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":219,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Milky Way; RADIUS; Stars; Scale height; Population; Radial velocity; Disc; Stellar population","score_opus":0.00621587056369702,"score_gpt":0.20989592026131249,"score_spread":0.20368004969761547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2203175835","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938047,0.000055493492,0.000060972736,0.000007961856,3.2786434e-7,8.378891e-7,0.0001542258,0.0000027382455,0.00033689398],"genre_scores_gemma":[0.9995528,0.000016506836,0.000056513567,0.0000021100675,0.0000011372218,7.8794324e-7,0.00025714503,0.0000014924483,0.0001115173],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998479,0.000024109086,0.000012536492,0.00005493415,0.00003452222,0.00002599629],"domain_scores_gemma":[0.99901235,0.00021701104,0.00026490117,0.00009009078,0.00027841737,0.00013726192],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002451658,0.00011651244,0.00017682352,0.0016400518,0.00020381663,0.0008260879,0.000268382,0.00022174533,0.0012657691],"category_scores_gemma":[0.0013957341,0.00010338093,0.00011649923,0.00087787677,0.00024879188,0.00039258742,0.0004907402,0.00010520883,0.0004339431],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037081456,0.000009645548,0.9933248,0.0000069634134,0.000030448897,0.000036015965,0.00014803867,0.00039285945,0.002998847,0.0001497223,0.0000670686,0.0027985882],"study_design_scores_gemma":[0.0000011513234,0.000008671344,0.9989624,0.0000014613231,0.0000037515192,0.00004705219,0.000079021775,0.0005764939,0.00016447468,0.000059081714,0.00009489244,0.0000015272659],"about_ca_topic_score_codex":0.0031887917,"about_ca_topic_score_gemma":0.002947767,"teacher_disagreement_score":0.0031887917,"about_ca_system_score_codex":0.0002978687,"about_ca_system_score_gemma":0.00008066454,"threshold_uncertainty_score":0.006340444},"labels":[],"label_agreement":null},{"id":"W2204123482","doi":"10.3847/0004-637x/823/1/19","title":"THE EXTENDED HALO OF CENTAURUS A: UNCOVERING SATELLITES, STREAMS, AND SUBSTRUCTURES*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":221,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Astrophysics; Centaurus A; Astronomy; Surface brightness; Local Group; Dwarf galaxy; Galaxy; Milky Way; Red-giant branch; Population; Globular cluster; Active galactic nucleus","score_opus":0.0047153362760847225,"score_gpt":0.1972387133828049,"score_spread":0.19252337710672018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2204123482","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983961,0.00035005657,0.0001651588,0.00001885731,0.0000019710521,0.0000018419629,0.00034007008,0.00002100177,0.0007047699],"genre_scores_gemma":[0.9993425,0.00007698553,0.00020682973,0.000007985834,0.0000042852716,8.9946076e-7,0.00026928846,0.0000029324076,0.00008826552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999473,0.0000045465185,0.0000033096917,0.000017064942,0.000011169645,0.000016585462],"domain_scores_gemma":[0.99966466,0.00003410665,0.000076218035,0.000046005243,0.000033648656,0.00014531722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001247949,0.00014491488,0.00013361442,0.0017333118,0.00029217286,0.0005092555,0.00016562987,0.000111773785,0.001343342],"category_scores_gemma":[0.00026134725,0.00007999671,0.00014319799,0.00093472074,0.00025855974,0.00024276647,0.00090401387,0.000110886496,0.00033391896],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011897435,0.000016011267,0.95557404,0.000046692356,0.00006232119,0.00039660864,0.0005571597,0.00024592507,0.027514217,0.00019621766,0.00038045534,0.014891395],"study_design_scores_gemma":[0.0000018560069,0.00001838076,0.9973907,0.0000071973436,0.000012544695,0.00031794733,0.0002501473,0.0002339648,0.00075989607,0.000109697256,0.0008941079,0.0000035586309],"about_ca_topic_score_codex":0.0042097713,"about_ca_topic_score_gemma":0.006874239,"teacher_disagreement_score":0.0042097713,"about_ca_system_score_codex":0.00016797564,"about_ca_system_score_gemma":0.000107714,"threshold_uncertainty_score":0.008370519},"labels":[],"label_agreement":null},{"id":"W2206917439","doi":"10.1088/0004-637x/793/1/51","title":"KINEMATIC MODELING OF THE MILKY WAY USING THE RAVE AND GCS STELLAR SURVEYS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":132,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Milky Way; Stellar kinematics; Kinematics; Astronomy; Astrophysics; Stars; Classical mechanics","score_opus":0.0212118237015976,"score_gpt":0.23141340441903008,"score_spread":0.21020158071743247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2206917439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9651389,0.00022494399,0.031991445,0.00013239775,0.0000056647687,0.000030028563,0.0009843307,0.00021807184,0.0012743052],"genre_scores_gemma":[0.98903835,0.00015229682,0.008696534,0.000020518544,0.000010051724,0.000033877208,0.001231054,0.000053422016,0.0007638771],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993875,0.00022898051,0.000038401347,0.00020658513,0.000070570284,0.000067984874],"domain_scores_gemma":[0.99811894,0.00069239445,0.00052989845,0.0003344697,0.0002380383,0.0000862282],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019465532,0.00038430453,0.00054183777,0.0012933539,0.00031299365,0.00125954,0.0011556839,0.0005390944,0.0006726775],"category_scores_gemma":[0.006200108,0.0004847192,0.00080790883,0.0010695186,0.00044915508,0.0012465008,0.00070039736,0.0003470117,0.0003098829],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000084263746,0.00003994762,0.33287156,0.000030194735,0.00015128731,0.0001702561,0.00046389134,0.64836085,0.001258242,0.006563855,0.00033548172,0.009670249],"study_design_scores_gemma":[0.000029367076,0.00008094139,0.1451426,0.000033773616,0.000061853054,0.00018913827,0.00015551428,0.8454272,0.0007474923,0.0056933067,0.00237917,0.0000595607],"about_ca_topic_score_codex":0.026916144,"about_ca_topic_score_gemma":0.016916966,"teacher_disagreement_score":0.026916144,"about_ca_system_score_codex":0.0009158624,"about_ca_system_score_gemma":0.0005776698,"threshold_uncertainty_score":0.05351895},"labels":[],"label_agreement":null},{"id":"W2207413084","doi":"10.1088/0004-637x/813/1/15","title":"3D MODELING OF GJ1214B’S ATMOSPHERE: VERTICAL MIXING DRIVEN BY AN ANTI-HADLEY CIRCULATION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Hadley cell; Downwelling; Equator; Atmosphere (unit); Haze; Atmospheric sciences; Metallicity; Atmospheric circulation; Physics; Astrophysics; Geology; Upwelling; General Circulation Model; Latitude; Meteorology; Astronomy; Climate change; Stars","score_opus":0.018947732849899132,"score_gpt":0.231537603709618,"score_spread":0.21258987085971887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2207413084","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9773053,0.00039358737,0.010288155,0.0007179714,0.00007756923,0.000041988173,0.0017180749,0.0003598898,0.00909754],"genre_scores_gemma":[0.9943211,0.00015621187,0.0030438453,0.00008383616,0.000041099374,0.0000354584,0.000742103,0.000050965235,0.0015253336],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991274,0.000025852622,0.000003890081,0.000019167786,0.000012688648,0.00002561716],"domain_scores_gemma":[0.99981624,0.000053991404,0.000033413653,0.000012027296,0.00002886982,0.00005556828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001617858,0.0006961106,0.0005016661,0.00046315775,0.00052792707,0.0009760155,0.0008024792,0.0016283239,0.0014770848],"category_scores_gemma":[0.00054515974,0.0003843137,0.0011397174,0.00037919346,0.000602811,0.00038341695,0.00065515976,0.0006147138,0.00020335287],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008125516,0.00004704792,0.007379658,0.000019991361,0.0000425895,0.00013497651,0.00004879973,0.98674124,0.002919378,0.0014633994,0.00036384346,0.0007578915],"study_design_scores_gemma":[0.000024494215,0.000010920829,0.002342362,0.0000024809653,0.0000072001803,0.000009136885,0.000014878299,0.9970741,0.00006824172,0.00022331106,0.00021634805,0.00000644726],"about_ca_topic_score_codex":0.08088187,"about_ca_topic_score_gemma":0.028542811,"teacher_disagreement_score":0.08088187,"about_ca_system_score_codex":0.0011207765,"about_ca_system_score_gemma":0.0006866571,"threshold_uncertainty_score":0.16082215},"labels":[],"label_agreement":null},{"id":"W2207892168","doi":"10.3847/0004-637x/817/2/162","title":"NEPTUNE’S DYNAMIC ATMOSPHERE FROM KEPLER K2 OBSERVATIONS: IMPLICATIONS FOR BROWN DWARF LIGHT CURVE ANALYSES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science Mission Directorate; Space Telescope Science Institute; California Institute of Technology; W. M. Keck Foundation; National Aeronautics and Space Administration","keywords":"Light curve; Brown dwarf; Neptune; Brightness; Context (archaeology); Planet; Exoplanet; Atmosphere (unit)","score_opus":0.03800110750658001,"score_gpt":0.28636855451825505,"score_spread":0.24836744701167504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2207892168","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947232,0.00022129317,0.0014605364,0.00008076435,0.0000049532887,0.000007958576,0.0006845063,0.000049751874,0.0027670132],"genre_scores_gemma":[0.99868554,0.000048414266,0.00073032605,0.000008728196,0.000006906659,0.0000023302853,0.00039708844,0.0000152682,0.00010531363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985075,0.00003632162,0.000015690295,0.000043441614,0.000029658697,0.000024057776],"domain_scores_gemma":[0.9988256,0.00045704076,0.00020494331,0.0001803195,0.00014597748,0.00018610292],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005061093,0.00023216849,0.00019528905,0.0011689055,0.0003697015,0.0010949242,0.00028478826,0.00015686669,0.00079046865],"category_scores_gemma":[0.0023142365,0.00010440032,0.0001918911,0.0010500301,0.0002378116,0.0006037174,0.00057955144,0.0002647788,0.00024034362],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039191128,0.000028855782,0.9517649,0.000043934066,0.00006404085,0.0003270342,0.0004676568,0.0020445,0.022300493,0.00043746846,0.00037680037,0.021752417],"study_design_scores_gemma":[0.0000053942667,0.000020844216,0.99118036,0.000008844745,0.000018328397,0.0001112303,0.00027034004,0.0045612836,0.00255069,0.00035234602,0.0009140951,0.0000062451186],"about_ca_topic_score_codex":0.0093173385,"about_ca_topic_score_gemma":0.010475308,"teacher_disagreement_score":0.0093173385,"about_ca_system_score_codex":0.00044249953,"about_ca_system_score_gemma":0.00020611152,"threshold_uncertainty_score":0.018526196},"labels":[],"label_agreement":null},{"id":"W2208707882","doi":"10.3847/0004-637x/817/2/183","title":"PLASMA-WAVE GENERATION IN A DYNAMIC SPACETIME","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Binary number; Isotropy; Electromagnetic radiation; Binary black hole; Collimated light; Component (thermodynamics); Radiation; Superluminal motion","score_opus":0.016439876162737337,"score_gpt":0.22636257400288118,"score_spread":0.20992269784014383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2208707882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8598491,0.00029292784,0.12550238,0.0002174272,0.00004760289,0.000032742053,0.000059064376,0.00019179759,0.013806919],"genre_scores_gemma":[0.9926112,0.00006147653,0.00650735,0.00002112464,0.000016301361,0.000010518296,0.000027641414,0.000011530505,0.0007327715],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999168,0.000020358058,0.000002534127,0.000018615408,0.000028902532,0.000012877264],"domain_scores_gemma":[0.9998598,0.000024347199,0.00003609026,0.000020765847,0.000023328996,0.00003558445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017764042,0.00030406608,0.00030230806,0.0004388993,0.00040962428,0.00061484834,0.0004775476,0.00030200268,0.000996349],"category_scores_gemma":[0.0006480712,0.00018606958,0.00028474917,0.00020692105,0.000733849,0.00091988407,0.00089896447,0.00034300474,0.000119308344],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003158783,0.000120898534,0.009548314,0.00015486106,0.0001044526,0.0012267606,0.00063033594,0.2088204,0.13322724,0.63107383,0.00088150665,0.013895551],"study_design_scores_gemma":[0.00012636546,0.00015244704,0.0070806188,0.000009095292,0.000020544583,0.0005931478,0.000103443905,0.9096288,0.0072792326,0.07268463,0.0022739882,0.00004774664],"about_ca_topic_score_codex":0.00034059118,"about_ca_topic_score_gemma":0.0001281093,"teacher_disagreement_score":0.000996349,"about_ca_system_score_codex":0.0004110838,"about_ca_system_score_gemma":0.00013962477,"threshold_uncertainty_score":0.0033331513},"labels":[],"label_agreement":null},{"id":"W2208815456","doi":"10.1088/0004-637x/815/1/38","title":"CONSTRAINED EVOLUTION OF A RADIALLY MAGNETIZED PROTOPLANETARY DISK: IMPLICATIONS FOR PLANETARY MIGRATION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Protoplanetary disk; Physics; Debris disk; Magnetorotational instability; Planet; Astrophysics; Formation and evolution of the Solar System; Planetary migration; Thick disk; Accretion (finance); Minimum mass; Angular momentum; Magnetic field; Thin disk; Planetary system; Magnetohydrodynamics; Stars; Galaxy","score_opus":0.016838194178750248,"score_gpt":0.2444555583980688,"score_spread":0.22761736421931855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2208815456","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9829153,0.0008063206,0.0064412723,0.0015009987,0.000040407907,0.000026378515,0.0003957389,0.00006540624,0.007808109],"genre_scores_gemma":[0.99819106,0.00018834039,0.00088683114,0.00006388396,0.000029533547,0.00001096055,0.00008323319,0.000026258815,0.00052001333],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999342,0.000016761169,0.0000027017197,0.000018924655,0.00000609216,0.000021278496],"domain_scores_gemma":[0.99976236,0.00006330655,0.000061106606,0.000021635855,0.000019577856,0.000071995615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020853881,0.000626042,0.0005734704,0.00025376125,0.0007797936,0.0018056879,0.001148535,0.0014680072,0.001538342],"category_scores_gemma":[0.0012503868,0.00036430306,0.00054596283,0.0002357626,0.0008788468,0.0012009873,0.0011013042,0.00073112635,0.00020583502],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046900267,0.00017768836,0.11687973,0.00012258982,0.0001474924,0.0028791693,0.00041203666,0.81162596,0.014845987,0.044731922,0.0014942406,0.0062141684],"study_design_scores_gemma":[0.00011427712,0.00012014886,0.054663613,0.000031097603,0.00004645029,0.0003740187,0.00040580324,0.92114055,0.0007688328,0.020844733,0.0014167726,0.00007363847],"about_ca_topic_score_codex":0.012413545,"about_ca_topic_score_gemma":0.0047719376,"teacher_disagreement_score":0.012413545,"about_ca_system_score_codex":0.0012966662,"about_ca_system_score_gemma":0.00044517746,"threshold_uncertainty_score":0.024682581},"labels":[],"label_agreement":null},{"id":"W2211953746","doi":"10.1086/308464","title":"Line Oscillator Strength Measurements in the 0–0 Band of the \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $c^{\\prime }_{4}{}^{1}\\Sigma ^{+}_{u}arrow X{}^{1}\\Sigma ^{+}_{g}$ \\end{document} Transition of N \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $_{2}$ \\end{document}","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gyrotron and Vacuum Electronics Research","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Steacie Institute for Molecular Sciences","funders":"","keywords":"Line (geometry); Combinatorics; Physics; Mathematics; Geometry","score_opus":0.020255023928163855,"score_gpt":0.26997036440494593,"score_spread":0.24971534047678207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2211953746","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04137093,0.00048747667,0.066570684,0.0013869765,0.0022478986,0.00030210998,0.032884352,0.03858665,0.8161629],"genre_scores_gemma":[0.16365625,0.00058160594,0.044802535,0.0010097797,0.00030472374,0.0003682055,0.040756747,0.03864156,0.7098787],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99955004,0.00003327522,0.000014308819,0.00011659338,0.00023552714,0.00005019523],"domain_scores_gemma":[0.99921227,0.0001462383,0.00005161025,0.00024003134,0.0002804204,0.00006947303],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00047201704,0.0005765208,0.00028332853,0.0009075493,0.00075560436,0.0013705009,0.0010436553,0.00089049013,0.28812975],"category_scores_gemma":[0.001679315,0.0004515004,0.0005041881,0.00080797315,0.0002731893,0.001557645,0.00079285225,0.0011931633,0.18590781],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055742014,0.00021101827,0.002711467,0.0002898871,0.00003554965,0.00022793331,0.0002998735,0.0008375412,0.123739086,0.008636527,0.7105698,0.15188394],"study_design_scores_gemma":[0.00005714278,0.000093656476,0.0065744794,0.00009302544,0.000031705113,0.00016732575,0.00010737482,0.003475777,0.13988437,0.0021233945,0.8473248,0.00006695976],"about_ca_topic_score_codex":0.002743418,"about_ca_topic_score_gemma":0.0051366594,"teacher_disagreement_score":0.71187025,"about_ca_system_score_codex":0.0008879141,"about_ca_system_score_gemma":0.00050177344,"threshold_uncertainty_score":0.96389},"labels":[],"label_agreement":null},{"id":"W2214468854","doi":"10.1088/0004-637x/806/2/254","title":"BANYAN. VI. DISCOVERY OF A COMPANION AT THE BROWN DWARF/PLANET-MASS LIMIT TO A TUCANA–HOROLOGIUM M DWARF","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"Brown dwarf; Planet; Proper motion; Diagram; Planetary mass; Direct imaging; Joins","score_opus":0.019794153114713792,"score_gpt":0.23177816940395962,"score_spread":0.21198401628924582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2214468854","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9453852,0.00185638,0.00086183875,0.0005457849,0.00010035069,0.00004575504,0.0017958923,0.00018139859,0.049227353],"genre_scores_gemma":[0.9851217,0.00034147562,0.0011474896,0.00024289946,0.000032569893,0.00001344399,0.0023745245,0.000018880719,0.010707037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998845,0.0000031747265,0.0000024488395,0.000040422023,0.000033438468,0.000035953733],"domain_scores_gemma":[0.99986434,0.000007473322,0.000027148233,0.000011730206,0.00003207366,0.0000572137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013084014,0.00022422943,0.00019624493,0.0007037652,0.0022286833,0.0010071459,0.0005249145,0.0006658137,0.004239739],"category_scores_gemma":[0.00020439754,0.00012529222,0.00010253894,0.0005254947,0.00034500213,0.0002450326,0.00086291356,0.00037482815,0.0015741618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010194066,0.0002404617,0.44164315,0.00031872684,0.000093783216,0.032544766,0.0016256525,0.00061345834,0.37582585,0.0073385136,0.016550872,0.12218528],"study_design_scores_gemma":[0.000039462953,0.00014986571,0.8177298,0.00008947618,0.0000642234,0.015115997,0.0011705685,0.0013353603,0.03812535,0.0016413907,0.12449939,0.000039186107],"about_ca_topic_score_codex":0.050362885,"about_ca_topic_score_gemma":0.07541789,"teacher_disagreement_score":0.050362885,"about_ca_system_score_codex":0.0012091001,"about_ca_system_score_gemma":0.00088930654,"threshold_uncertainty_score":0.1001395},"labels":[],"label_agreement":null},{"id":"W2214860362","doi":"10.1088/0004-637x/761/2/96","title":"ACCELERATION OF VERY SMALL DUST GRAINS DUE TO RANDOM CHARGE FLUCTUATIONS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Acceleration; Electron; Photoelectric effect; Ionization; Debye length; Charge (physics); Ion; Interstellar medium","score_opus":0.021381924007712744,"score_gpt":0.2500670210187785,"score_spread":0.22868509701106574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2214860362","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921103,0.00013006537,0.00617567,0.000064712985,0.000013086471,0.000010386279,0.000026819525,0.000043093878,0.0014258565],"genre_scores_gemma":[0.99934775,0.000044182158,0.00041299564,0.000009797095,0.0000058842334,0.0000032251116,0.000015264694,0.000006926283,0.00015407622],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999193,0.000013341805,0.0000030975143,0.00001315828,0.000018178871,0.000032841395],"domain_scores_gemma":[0.9995772,0.00015914868,0.000109928835,0.000031482374,0.00004073788,0.000081447986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014932621,0.00025239406,0.00026074942,0.00031527667,0.00038327242,0.0005040161,0.00037655103,0.00038646275,0.0005240264],"category_scores_gemma":[0.0009676445,0.0001953086,0.0003579031,0.0002747081,0.00065202126,0.00043195442,0.00037720974,0.00026760192,0.000061334176],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001747892,0.00007703773,0.01898794,0.000048390462,0.00010323258,0.00081134355,0.00010885965,0.9448552,0.02462419,0.0066529755,0.00029115938,0.0032647774],"study_design_scores_gemma":[0.0000268051,0.0000507555,0.00557822,0.0000020393074,0.00001537033,0.00007102148,0.000027525844,0.9907733,0.0020633282,0.0012090589,0.00017230566,0.000010284559],"about_ca_topic_score_codex":0.006304768,"about_ca_topic_score_gemma":0.002315137,"teacher_disagreement_score":0.006304768,"about_ca_system_score_codex":0.0005416764,"about_ca_system_score_gemma":0.00027615685,"threshold_uncertainty_score":0.012536168},"labels":[],"label_agreement":null},{"id":"W2214954459","doi":"10.3847/0004-637x/823/2/122","title":"3.6 AND 4.5 μm SPITZER PHASE CURVES OF THE HIGHLY IRRADIATED HOT JUPITERS WASP-19b AND HAT-P-7b","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":144,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Hot Jupiter; Astrophysics; Physics; Planet; Atmospheric escape; Atmospheric sciences; Astronomy; Exoplanet","score_opus":0.009401271199071153,"score_gpt":0.22309746380449966,"score_spread":0.2136961926054285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2214954459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997113,0.00006178261,0.0003378514,0.000029528475,0.0000049449027,0.000007955906,0.0009802508,0.0000922372,0.0013724541],"genre_scores_gemma":[0.9970969,0.000029835435,0.0004421441,0.000013012847,0.000008603601,0.0000090379235,0.0021675953,0.00003064718,0.00020230307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994516,0.0000036637591,0.0000015939517,0.00001692802,0.000013170798,0.00001952873],"domain_scores_gemma":[0.9997491,0.000037304057,0.00007545954,0.000027347804,0.00004946228,0.00006136806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015050167,0.00032584128,0.0002059265,0.00090513215,0.0003089781,0.00029599803,0.00028624077,0.00040139304,0.001022622],"category_scores_gemma":[0.00034185758,0.00019616768,0.00040516668,0.0004464583,0.00021836259,0.00025141393,0.00029523706,0.00036225512,0.00023873488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017443926,0.00028326912,0.66188,0.00016325602,0.00031520726,0.00093108026,0.00082079356,0.0138515765,0.28816423,0.0009214456,0.0036280584,0.027296605],"study_design_scores_gemma":[0.000021411375,0.00006312731,0.98808086,0.0000052857713,0.000018762468,0.00007859881,0.00003999531,0.0064245774,0.004247057,0.000091645394,0.0009185793,0.0000098970795],"about_ca_topic_score_codex":0.004583364,"about_ca_topic_score_gemma":0.0046958197,"teacher_disagreement_score":0.004583364,"about_ca_system_score_codex":0.00045831705,"about_ca_system_score_gemma":0.000081184815,"threshold_uncertainty_score":0.009113371},"labels":[],"label_agreement":null},{"id":"W2215488956","doi":"10.1088/0004-637x/814/2/99","title":"FROM SOLAR TO STELLAR CORONA: THE ROLE OF WIND, ROTATION, AND MAGNETISM","year":2015,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Stellar magnetic field; Magnetic field; Astrophysics; Corona (planetary geology); Solar wind; Computational physics; Magnetic flux; Stellar rotation; Dipole model of the Earth's magnetic field; Coronal mass ejection; Stars; Interplanetary magnetic field","score_opus":0.006858340825470479,"score_gpt":0.222336767771957,"score_spread":0.2154784269464865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2215488956","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8489973,0.03664998,0.06857539,0.004149883,0.00046609418,0.000047765334,0.0010995304,0.0005846948,0.039429348],"genre_scores_gemma":[0.9893975,0.0048042564,0.0039923983,0.00015517442,0.000163698,0.000009540341,0.00025173125,0.00009441904,0.0011312723],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999434,0.000016148993,0.0000030528072,0.000018108936,0.0000133300955,0.0000058667324],"domain_scores_gemma":[0.9998841,0.000043531647,0.000020639438,0.000015569914,0.000018276638,0.000017869374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024015007,0.0002858865,0.00024914034,0.00022443691,0.00021082978,0.0011169858,0.0002788026,0.00035742339,0.001112583],"category_scores_gemma":[0.00080834236,0.000115305294,0.00017152983,0.0003254976,0.00036307,0.00089185516,0.00039553674,0.00036393202,0.00018699246],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003883639,0.00018465887,0.21901385,0.0013700054,0.00032686244,0.001481642,0.0017441702,0.20733057,0.04489195,0.1839038,0.020283345,0.3190807],"study_design_scores_gemma":[0.00008174625,0.00019905521,0.31998718,0.00030392673,0.00012396416,0.0008468479,0.00063905393,0.43117005,0.0036450468,0.15108863,0.09180932,0.000105234096],"about_ca_topic_score_codex":0.002374687,"about_ca_topic_score_gemma":0.0014659439,"teacher_disagreement_score":0.002374687,"about_ca_system_score_codex":0.00031933538,"about_ca_system_score_gemma":0.00014700137,"threshold_uncertainty_score":0.0047217607},"labels":[],"label_agreement":null},{"id":"W2218632722","doi":"10.1088/0004-637x/812/1/88","title":"STELLAR MASSES AND STAR FORMATION RATES OF LENSED, DUSTY, STAR-FORMING GALAXIES FROM THE SPT SURVEY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Star formation; Stellar mass; Galaxy; Redshift; Spectral energy distribution; COSMIC cancer database; Universe; Galaxy formation and evolution; Telescope","score_opus":0.026379279359918403,"score_gpt":0.2368594185519116,"score_spread":0.21048013919199318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2218632722","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99731606,0.00007056983,0.00032703442,0.000015155614,0.0000018514539,0.0000044429066,0.0013105901,0.000024444658,0.0009298063],"genre_scores_gemma":[0.99320316,0.00012445243,0.00088274723,0.000013469707,0.000015546135,0.000006846633,0.0054521924,0.000012762864,0.000288791],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981445,0.000014551991,0.000016520464,0.000053704087,0.00007373025,0.00002692003],"domain_scores_gemma":[0.9990182,0.00012909822,0.00036285684,0.00013163892,0.00019779029,0.00016037033],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033781398,0.00029341452,0.00021474375,0.0023238389,0.00026381545,0.00049868296,0.00027988042,0.00020534398,0.0015780793],"category_scores_gemma":[0.0011893411,0.00012806545,0.00027406585,0.0014475922,0.00023654208,0.00041083485,0.0005998782,0.0002998804,0.00049534277],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030874035,0.00001201573,0.98957235,0.00001242954,0.00003677094,0.00006584143,0.00020035732,0.0002775673,0.001982022,0.00007528282,0.0003090348,0.007425395],"study_design_scores_gemma":[0.0000013970823,0.000013827397,0.99882334,0.0000016445978,0.000009178903,0.00012513218,0.000036882346,0.00032690517,0.0003491176,0.000031888096,0.00027903236,0.0000016290005],"about_ca_topic_score_codex":0.0045437105,"about_ca_topic_score_gemma":0.0074144136,"teacher_disagreement_score":0.0045437105,"about_ca_system_score_codex":0.00024748783,"about_ca_system_score_gemma":0.00012342246,"threshold_uncertainty_score":0.009034574},"labels":[],"label_agreement":null},{"id":"W2220390127","doi":"10.1088/0004-637x/809/1/6","title":"NATURE’S STARSHIPS. II. SIMULATING THE SYNTHESIS OF AMINO ACIDS IN METEORITE PARENT BODIES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Meteorite; Planetesimal; Chondrite; Murchison meteorite; Parent body; Amino acid; Chemistry; Astrobiology; Abundance (ecology); Carbonaceous chondrite; Astrochemistry; Relative species abundance; Astrophysics; Physics; Solar System; Biology; Biochemistry; Ecology; Galaxy","score_opus":0.02278654077096639,"score_gpt":0.25362989863510393,"score_spread":0.23084335786413754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2220390127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7260997,0.0007630642,0.06273529,0.0017329009,0.001327282,0.00026123237,0.022076257,0.012570566,0.1724337],"genre_scores_gemma":[0.88718694,0.0004369394,0.06484027,0.0003896243,0.00009483322,0.00021008794,0.011195376,0.001218134,0.03442767],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999497,0.000010043299,0.0000025249658,0.00001657415,0.000012736619,0.000008455919],"domain_scores_gemma":[0.99983025,0.00004121963,0.00001523789,0.00002715958,0.000034109304,0.000052054005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016577666,0.00031532868,0.00021703022,0.00019234777,0.0003522092,0.00073632924,0.0007776509,0.0007824562,0.012622999],"category_scores_gemma":[0.0005963828,0.00022325327,0.00036148095,0.00038286854,0.00018066718,0.0006242144,0.00047245843,0.0005839054,0.002604898],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000532745,0.00033272294,0.055336095,0.00021662054,0.00014494905,0.00043151111,0.00034445844,0.82831264,0.004769017,0.018961566,0.052327447,0.0382902],"study_design_scores_gemma":[0.00012446083,0.00005813552,0.005080058,0.000015517055,0.00001884846,0.00006676594,0.000085273685,0.9399288,0.0016514749,0.005971585,0.04698762,0.00001153903],"about_ca_topic_score_codex":0.010887359,"about_ca_topic_score_gemma":0.016176928,"teacher_disagreement_score":0.012622999,"about_ca_system_score_codex":0.00046562968,"about_ca_system_score_gemma":0.000601058,"threshold_uncertainty_score":0.042228162},"labels":[],"label_agreement":null},{"id":"W2220519623","doi":"10.1088/0004-637x/806/1/17","title":"MORPHOLOGY AND KINEMATICS OF WARM MOLECULAR GAS IN THE NUCLEAR REGION OF ARP 220 AS REVEALED BY ALMA","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Redshift; Millimeter; Line (geometry); Kinematics; Galaxy; Emission spectrum; Velocity gradient; Plateau de Bure Interferometer","score_opus":0.009550372827374904,"score_gpt":0.21757391037191914,"score_spread":0.20802353754454425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2220519623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987484,0.000053927004,0.000081156155,0.000012036494,0.0000014769539,0.0000020709685,0.000090318914,0.000021275913,0.0009894362],"genre_scores_gemma":[0.99945194,0.000025422089,0.00022164948,0.000008387666,0.0000065992567,0.0000026944874,0.00016287486,0.0000055884448,0.000114952614],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992454,0.0000095529385,0.000003881937,0.000025529054,0.000017282244,0.000019109531],"domain_scores_gemma":[0.99980813,0.000020551686,0.000073413285,0.00002497168,0.000020659412,0.000052372277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009759192,0.00013221522,0.00018583094,0.0007857554,0.0003210381,0.0005955464,0.00035148702,0.00021939477,0.00058281946],"category_scores_gemma":[0.00035911918,0.00016388952,0.00012453979,0.0003716649,0.00021529564,0.0002836196,0.00039497868,0.0001853464,0.0002066066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006370719,0.00019185177,0.75204945,0.000059029586,0.000121528705,0.0016272638,0.0009780275,0.002690054,0.22153296,0.0011651333,0.00091630017,0.018031377],"study_design_scores_gemma":[0.000008984875,0.000062842526,0.9939015,0.000004195629,0.000019397083,0.0003052196,0.00015190912,0.0020486102,0.002489141,0.000102430466,0.0008961754,0.000009667342],"about_ca_topic_score_codex":0.0025895613,"about_ca_topic_score_gemma":0.0034904147,"teacher_disagreement_score":0.0025895613,"about_ca_system_score_codex":0.0002771095,"about_ca_system_score_gemma":0.0000691887,"threshold_uncertainty_score":0.005149007},"labels":[],"label_agreement":null},{"id":"W2221333501","doi":"10.3847/0004-637x/817/1/73","title":"FINDING, CHARACTERIZING, AND CLASSIFYING VARIABLE SOURCES IN MULTI-EPOCH SKY SURVEYS: QSOs AND RR LYRAE IN PS1 3π DATA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Centre National de la Recherche Scientifique; Deutsche Forschungsgemeinschaft; Queen's University Belfast; Durham University; York University; Space Telescope Science Institute; Carnegie Mellon University; Los Alamos National Laboratory; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Harvard University; Queen's University; Ohio State University; National Science Foundation; University Grants Commission; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; European Commission; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University","keywords":"RR Lyrae variable; QSOS; Sky; Light curve; Variable star; Amplitude; Sample (material)","score_opus":0.04745321395028253,"score_gpt":0.2700359404274088,"score_spread":0.2225827264771263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2221333501","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961515,0.00008157992,0.0020820345,0.000035713496,0.0000020370012,0.000013344585,0.0013178154,0.00008091117,0.00023506884],"genre_scores_gemma":[0.99363744,0.00004656391,0.0030739086,0.000012293576,0.0000068918307,0.000010854197,0.003070419,0.000015176299,0.00012649539],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967885,0.00005619847,0.000023599876,0.00009519262,0.00008595525,0.00006022429],"domain_scores_gemma":[0.9983211,0.0005158168,0.0005021096,0.00023966843,0.00021129858,0.00021007274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096749834,0.00022990225,0.00030543364,0.0030062262,0.00031484535,0.00054284994,0.0003159838,0.0002741351,0.0005858006],"category_scores_gemma":[0.0021022444,0.00013009657,0.0003802706,0.0015888028,0.00020142393,0.00041256638,0.0005883653,0.00030452327,0.00037724752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000074528725,0.000038151025,0.97497547,0.00002129744,0.000047268277,0.000064800355,0.00012147574,0.0034633554,0.0051731532,0.00015910123,0.000545158,0.015316414],"study_design_scores_gemma":[0.0000068308036,0.00002285299,0.98460495,0.0000059579443,0.000016931346,0.00005729609,0.00012716385,0.013187046,0.0012603042,0.00013084435,0.0005736676,0.0000060607895],"about_ca_topic_score_codex":0.010967737,"about_ca_topic_score_gemma":0.014714538,"teacher_disagreement_score":0.010967737,"about_ca_system_score_codex":0.00034482757,"about_ca_system_score_gemma":0.00029358605,"threshold_uncertainty_score":0.02180779},"labels":[],"label_agreement":null},{"id":"W2222668598","doi":"10.3847/0004-637x/820/2/111","title":"POINT SOURCE POLARIMETRY WITH THE GEMINI PLANET IMAGER: SENSITIVITY CHARACTERIZATION WITH T5.5 DWARF COMPANION HD 19467 B","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Livermore National Laboratory; NASA Exoplanet Science Institute; California Institute of Technology; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Brown dwarf; Exoplanet; Physics; Polarimetry; Polarization (electrochemistry); Surface gravity; Astrophysics; Planet; Stars; Optics; Scattering; Chemistry","score_opus":0.005491602250505255,"score_gpt":0.1867266689389092,"score_spread":0.18123506668840395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2222668598","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99760735,0.00006392179,0.0006753622,0.000012894018,0.00000277332,0.0000068218033,0.00060079584,0.00004884545,0.0009812831],"genre_scores_gemma":[0.9984517,0.000016783823,0.0006346659,0.000006794509,0.00000442106,0.0000020771467,0.000758478,0.000005742848,0.00011922091],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998908,0.000011256979,0.000004950358,0.000039838418,0.000028702092,0.00002434294],"domain_scores_gemma":[0.99985194,0.000022421687,0.000036824327,0.00002439684,0.000030286648,0.000034103283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001674559,0.00012447614,0.000115225484,0.0004508052,0.000209284,0.0003632213,0.00012931379,0.00018224127,0.00084381545],"category_scores_gemma":[0.00037216267,0.00008303591,0.00014525645,0.0004599675,0.00010986001,0.00021006208,0.00025921682,0.00012469687,0.00021135971],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000638936,0.000111917485,0.8131463,0.0000589654,0.00013265318,0.0003522928,0.00030857793,0.0035297398,0.15868974,0.0003833245,0.0014024838,0.021245185],"study_design_scores_gemma":[0.000009489814,0.00009713492,0.97799927,0.00000406435,0.000031384483,0.00021350812,0.00010055896,0.0065286364,0.0138411205,0.00008585169,0.0010817357,0.0000072541297],"about_ca_topic_score_codex":0.0073847915,"about_ca_topic_score_gemma":0.010554656,"teacher_disagreement_score":0.0073847915,"about_ca_system_score_codex":0.00022109594,"about_ca_system_score_gemma":0.00008526263,"threshold_uncertainty_score":0.014683604},"labels":[],"label_agreement":null},{"id":"W2223659637","doi":"10.1088/0004-637x/769/2/136","title":"MODELING THE NEAR-ULTRAVIOLET BAND OF GK STARS. III. DEPENDENCE ON ABUNDANCE PATTERN","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Stars; Abundance (ecology); Spectral line; Line (geometry); Spectral density; Stellar atmosphere; Wavelength; Atmospheric models","score_opus":0.01185392821071661,"score_gpt":0.21982922774586777,"score_spread":0.20797529953515115,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2223659637","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9053783,0.00017853924,0.07485708,0.00027056187,0.000053038777,0.000054721157,0.0031647156,0.0006671604,0.01537589],"genre_scores_gemma":[0.977201,0.000095831274,0.016876677,0.00011354142,0.00001644392,0.000047292302,0.0013721033,0.0001667042,0.004110463],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988854,0.000022709417,0.000005904928,0.000039024446,0.0000174629,0.000026242784],"domain_scores_gemma":[0.9998056,0.000050830244,0.000032958862,0.00004955394,0.000038860184,0.000022156588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017520097,0.00038824836,0.00023619052,0.0002630361,0.00020101127,0.000665926,0.00083909486,0.00061437587,0.0031956348],"category_scores_gemma":[0.0008332661,0.00022004967,0.0008204733,0.0003795922,0.00019423927,0.00075178046,0.00042005072,0.0004793226,0.0011664563],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010704785,0.00010318379,0.08237369,0.00008384704,0.00010795536,0.00015212505,0.00015509114,0.88874876,0.010229887,0.005458599,0.0013456324,0.01113415],"study_design_scores_gemma":[0.000022685375,0.000031668347,0.021297252,0.000011530965,0.00001945907,0.0000804001,0.00006744005,0.97036844,0.0023427808,0.003345227,0.002395697,0.000017388173],"about_ca_topic_score_codex":0.015027581,"about_ca_topic_score_gemma":0.011150137,"teacher_disagreement_score":0.015027581,"about_ca_system_score_codex":0.00046556638,"about_ca_system_score_gemma":0.00022695224,"threshold_uncertainty_score":0.029880226},"labels":[],"label_agreement":null},{"id":"W2225235405","doi":"10.3847/0004-637x/826/2/216","title":"DICKE’S SUPERRADIANCE IN ASTROPHYSICS. I. THE 21 cm LINE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Superradiance; Population inversion; Maser; Dephasing; Physics; Astrophysics; Coherence (philosophical gambling strategy); Population; Dipole; Computational physics; Quantum mechanics","score_opus":0.011923373470446664,"score_gpt":0.2224594912490882,"score_spread":0.21053611777864153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2225235405","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89320546,0.0134375375,0.04147085,0.002024753,0.00019096977,0.000020198599,0.00012834562,0.00007687753,0.04944496],"genre_scores_gemma":[0.99475044,0.00095651747,0.0030972508,0.000082281746,0.00009711084,0.0000035086236,0.000015472035,0.00000602505,0.0009915328],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998006,0.00006529731,0.000009846195,0.000050218878,0.00003767474,0.000036341073],"domain_scores_gemma":[0.99844223,0.00076357945,0.00042116072,0.00016699561,0.00010717032,0.00009895843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000652587,0.00020500612,0.00024535754,0.0013041326,0.0003970997,0.0006820991,0.00037968613,0.00036820158,0.0019750502],"category_scores_gemma":[0.0017923434,0.00011596489,0.00019643722,0.001061309,0.0018706305,0.0015123888,0.0007655253,0.00076933065,0.00019679773],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025786192,0.000064136424,0.053422995,0.00014105094,0.000048204794,0.0013788112,0.0010021196,0.0066564316,0.026453497,0.8451723,0.0013388656,0.0640637],"study_design_scores_gemma":[0.000031847725,0.00023045458,0.13095422,0.00007798063,0.000035410583,0.0026815932,0.0007877514,0.024173116,0.015478938,0.7611947,0.06424983,0.00010411263],"about_ca_topic_score_codex":0.0005014789,"about_ca_topic_score_gemma":0.0004157717,"teacher_disagreement_score":0.0019750502,"about_ca_system_score_codex":0.00043633793,"about_ca_system_score_gemma":0.00012815511,"threshold_uncertainty_score":0.0066072345},"labels":[],"label_agreement":null},{"id":"W2226333607","doi":"10.3847/0004-637x/828/1/57","title":"DICKE’S SUPERRADIANCE IN ASTROPHYSICS. II. THE OH 1612 MHz LINE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Superradiance; Maser; Population inversion; Stars; Line (geometry); Spectral line; Population","score_opus":0.01162331280768827,"score_gpt":0.23448012255172385,"score_spread":0.22285680974403557,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2226333607","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7388351,0.07982979,0.068474256,0.005085766,0.0014686616,0.00006276908,0.0002724915,0.000106579086,0.1058646],"genre_scores_gemma":[0.9838365,0.0052748546,0.0063857683,0.00028860106,0.00047640526,0.000014487525,0.000040057836,0.000011511643,0.003671934],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99984396,0.00004147786,0.00000919113,0.00004085412,0.000028597851,0.000035961057],"domain_scores_gemma":[0.9993943,0.00026029302,0.00018799049,0.000056220746,0.000044288714,0.00005681108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044894702,0.00027896825,0.00027658872,0.001514056,0.0004712265,0.0009541438,0.00039859593,0.00045557707,0.0018885001],"category_scores_gemma":[0.0007637678,0.00014441786,0.00024473327,0.0013353379,0.0020846059,0.0015548147,0.0008436446,0.00072765816,0.00042319536],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016879333,0.000091005335,0.041732233,0.00019326761,0.000037307545,0.0018966962,0.0009884615,0.0026367293,0.014988456,0.85283077,0.0036719213,0.08076445],"study_design_scores_gemma":[0.000032270716,0.00027432307,0.09404311,0.00012855374,0.000048481008,0.0045788977,0.0012182752,0.016063131,0.012799272,0.69180197,0.17890617,0.00010555058],"about_ca_topic_score_codex":0.0005234929,"about_ca_topic_score_gemma":0.00043729672,"teacher_disagreement_score":0.0018885001,"about_ca_system_score_codex":0.00046369582,"about_ca_system_score_gemma":0.00014779322,"threshold_uncertainty_score":0.0063177347},"labels":[],"label_agreement":null},{"id":"W2226728599","doi":"10.1088/0004-637x/808/1/98","title":"NEAR-INFRARED EXTINCTION DUE TO COOL SUPERNOVA DUST IN CASSIOPEIA A","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cassiopeia A; Ejecta; Extinction (optical mineralogy); Supernova remnant; Cosmic dust; Supernova; Flux (metallurgy); Grain size","score_opus":0.020511696313769232,"score_gpt":0.24898470276433554,"score_spread":0.2284730064505663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2226728599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994804,0.000040543106,0.000048468053,0.000004741087,6.646883e-7,0.0000011531549,0.000067640794,0.0000073468595,0.00034910464],"genre_scores_gemma":[0.9993352,0.0000649653,0.00014743544,0.000008310849,0.0000032465432,0.0000032747064,0.00028123916,0.0000054350853,0.00015098606],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991167,0.000005536175,0.000004505581,0.00003836993,0.000020549345,0.000019351251],"domain_scores_gemma":[0.9995921,0.00006633719,0.00014252853,0.000045004206,0.00007042861,0.00008365359],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016970986,0.00028566824,0.00019713746,0.0008184162,0.00049521675,0.00035664733,0.00020929576,0.00019632804,0.00050808844],"category_scores_gemma":[0.0004390192,0.0001671936,0.0001755292,0.00045900675,0.000284123,0.00014884656,0.0004064526,0.00022718,0.00010846951],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034693882,0.000053137297,0.8002739,0.000046608737,0.00014192355,0.0008667893,0.0004676861,0.0012002453,0.19098929,0.00013685384,0.00022003971,0.0052566286],"study_design_scores_gemma":[0.0000034738928,0.000023511777,0.99712175,0.0000018168104,0.000012435174,0.000095723575,0.000031514308,0.00034775143,0.0021830169,0.000015876747,0.00016090476,0.0000022318673],"about_ca_topic_score_codex":0.013694494,"about_ca_topic_score_gemma":0.013967336,"teacher_disagreement_score":0.013694494,"about_ca_system_score_codex":0.00047382855,"about_ca_system_score_gemma":0.000114708266,"threshold_uncertainty_score":0.027229548},"labels":[],"label_agreement":null},{"id":"W2229740181","doi":"10.3847/0004-637x/818/2/182","title":"CONSTRAINTS ON FEEDBACK IN THE LOCAL UNIVERSE: THE RELATION BETWEEN STAR FORMATION AND AGN ACTIVITY IN EARLY-TYPE GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Radio galaxy; Star formation; Luminous infrared galaxy; Elliptical galaxy; Galaxy; Peculiar galaxy; Brightest cluster galaxy; Galaxy cluster","score_opus":0.011354370406172888,"score_gpt":0.21239008362588035,"score_spread":0.20103571321970748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2229740181","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996394,0.00005911922,0.000072176554,0.0000057948964,2.8528237e-7,7.4539014e-7,0.0000752197,0.0000019237573,0.00014534431],"genre_scores_gemma":[0.9998129,0.000016621549,0.000031652264,0.0000025070003,0.0000014178513,5.0632053e-7,0.00008832307,7.4168577e-7,0.000045293702],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996902,0.000097410084,0.000026854354,0.00006178171,0.00006621185,0.000057523604],"domain_scores_gemma":[0.9945267,0.0025532958,0.0013562565,0.00038638213,0.00036088112,0.0008164077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008258306,0.00019277116,0.0004932128,0.0012953554,0.0002580785,0.00076477067,0.0003716383,0.00027342432,0.0022654266],"category_scores_gemma":[0.0040938105,0.00014527916,0.00023666752,0.0009610233,0.000431828,0.0004486129,0.00047761868,0.00020222775,0.00026055705],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047870344,0.000013491857,0.9970913,0.0000070891333,0.000028987879,0.000030460355,0.000067202054,0.00015600273,0.0013859461,0.000032239903,0.000009927071,0.001129403],"study_design_scores_gemma":[0.0000010018632,0.00001651794,0.99951303,0.0000010460699,0.0000078784315,0.000033597797,0.00004890619,0.00021485586,0.0001116496,0.000026409696,0.00002406982,9.934337e-7],"about_ca_topic_score_codex":0.0059220404,"about_ca_topic_score_gemma":0.009713663,"teacher_disagreement_score":0.0059220404,"about_ca_system_score_codex":0.00025311654,"about_ca_system_score_gemma":0.00014379731,"threshold_uncertainty_score":0.011775136},"labels":[],"label_agreement":null},{"id":"W2230481379","doi":"10.3847/0004-637x/818/1/88","title":"ON R − W1 AS A DIAGNOSTIC TO DISCOVER OBSCURED ACTIVE GALACTIC NUCLEI IN WIDE-AREA X-RAY SURVEYS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Algorithm; Computer science","score_opus":0.012723301622189542,"score_gpt":0.23974800501110005,"score_spread":0.2270247033889105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2230481379","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99641705,0.0001296866,0.0009914419,0.00003366682,0.0000033773053,0.000009685638,0.00045893042,0.000085543994,0.0018707421],"genre_scores_gemma":[0.9987943,0.000024750716,0.0006541082,0.0000104961355,0.0000052744576,0.0000027278118,0.00034564294,0.0000095195,0.00015315901],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99935585,0.00021954594,0.000044048982,0.00013912469,0.00014913292,0.00009226421],"domain_scores_gemma":[0.9941561,0.0025477845,0.001808634,0.0004962675,0.00043725033,0.00055397657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017863825,0.00030749876,0.00021185102,0.003040904,0.00022822298,0.00095109234,0.00046992788,0.00031011252,0.0015324303],"category_scores_gemma":[0.005109975,0.000108940854,0.00022283303,0.0011402327,0.00054698845,0.0007708924,0.0008280827,0.0002870976,0.0006015999],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011438765,0.00001659472,0.99165404,0.000014354138,0.000033979177,0.000032783646,0.000045990004,0.0007836646,0.0017719284,0.000109826804,0.00017375375,0.0052486486],"study_design_scores_gemma":[0.00000546831,0.00007180007,0.99339676,0.000010914619,0.000014410815,0.00007191877,0.00015251448,0.0049782055,0.00090613874,0.00009325283,0.00029418216,0.000004364351],"about_ca_topic_score_codex":0.0030860412,"about_ca_topic_score_gemma":0.0063111996,"teacher_disagreement_score":0.0030860412,"about_ca_system_score_codex":0.0002344155,"about_ca_system_score_gemma":0.00015666474,"threshold_uncertainty_score":0.009447396},"labels":[],"label_agreement":null},{"id":"W2230763664","doi":"10.3847/0004-637x/823/1/37","title":"DETECTION OF LENSING SUBSTRUCTURE USING ALMA OBSERVATIONS OF THE DUSTY GALAXY SDP.81","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":329,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University","funders":"","keywords":"Substructure; Gravitational lens; Galaxy; Dark matter; Population; Halo; Weak gravitational lensing; Interferometry","score_opus":0.016264976853500902,"score_gpt":0.21253406731659447,"score_spread":0.19626909046309357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2230763664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985832,0.000029864326,0.00041613023,0.000023373252,0.000001324608,0.0000037544714,0.00029833397,0.000026066864,0.0006178948],"genre_scores_gemma":[0.9989579,0.000014445582,0.00056905893,0.000007867945,0.000003810616,0.0000031469633,0.00037173857,0.0000034449893,0.000068640125],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975604,0.000031168383,0.000013907564,0.00008069668,0.00007759206,0.000040520415],"domain_scores_gemma":[0.99895096,0.00020171337,0.0003534138,0.00018780086,0.000118610464,0.00018740584],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042952015,0.00027251034,0.00028312032,0.0011266313,0.0003456158,0.00067151105,0.00032045098,0.00023716695,0.00069541135],"category_scores_gemma":[0.0010534493,0.00020840524,0.00026018173,0.00065975165,0.00025284663,0.0003724997,0.00072231406,0.00028713263,0.0002694224],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016173034,0.00004604828,0.94966453,0.00003377473,0.0001467579,0.00027878294,0.00026019424,0.0022447738,0.03861209,0.00041954455,0.00030618958,0.007825561],"study_design_scores_gemma":[0.0000102860595,0.00005656524,0.98812276,0.0000049555383,0.00003204796,0.00012326032,0.00007753437,0.0073323552,0.0034391927,0.00019941312,0.00059305906,0.00000852458],"about_ca_topic_score_codex":0.0031316916,"about_ca_topic_score_gemma":0.005494048,"teacher_disagreement_score":0.0031316916,"about_ca_system_score_codex":0.0004414275,"about_ca_system_score_gemma":0.00017184841,"threshold_uncertainty_score":0.0062268972},"labels":[],"label_agreement":null},{"id":"W2232121806","doi":"10.3847/0004-637x/818/1/21","title":"INTERRUPTED BINARY MASS TRANSFER IN STAR CLUSTERS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Globular cluster; Star cluster; Binary number; Cluster (spacecraft); Binary star; Stellar evolution; Stars; Stellar mass; Star formation; Star (game theory)","score_opus":0.011673425660792885,"score_gpt":0.22695632828505077,"score_spread":0.2152829026242579,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2232121806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99848574,0.000027370143,0.0010771932,0.000013852495,0.0000018764163,0.0000029081302,0.00002798361,0.000021318205,0.00034173435],"genre_scores_gemma":[0.99965465,0.0000120341865,0.00018802728,0.0000023376772,0.0000012739778,0.000002387679,0.000038256458,0.000004847999,0.00009618755],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998485,0.000026116799,0.000006045069,0.000047413483,0.00003499056,0.00003683277],"domain_scores_gemma":[0.99878496,0.000557185,0.0002252441,0.00014018468,0.00012559291,0.00016674194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039944475,0.00022845223,0.0003825699,0.0005941576,0.00055786996,0.00080527406,0.00070154096,0.00041299907,0.0013042974],"category_scores_gemma":[0.0030314012,0.00019827417,0.00027690956,0.0004797772,0.00065429957,0.00053067313,0.0007441449,0.0004339915,0.000103084036],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029849514,0.00012937252,0.10918081,0.000037277692,0.00008124171,0.00029506834,0.00022852805,0.8695176,0.007652871,0.0077640065,0.00034126264,0.0044734897],"study_design_scores_gemma":[0.000042540043,0.00012819473,0.041660063,0.0000056462404,0.000023004046,0.00012235202,0.000098736935,0.95044464,0.003253308,0.0037974387,0.00040482567,0.000019229381],"about_ca_topic_score_codex":0.0047065513,"about_ca_topic_score_gemma":0.0022949544,"teacher_disagreement_score":0.0047065513,"about_ca_system_score_codex":0.0010615264,"about_ca_system_score_gemma":0.0003388712,"threshold_uncertainty_score":0.009358346},"labels":[],"label_agreement":null},{"id":"W2232556026","doi":"10.3847/0004-637x/823/2/98","title":"SIMULATIONS OF THE PAIRWISE KINEMATIC SUNYAEV–ZEL’DOVICH SIGNAL","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pairwise comparison; Cosmic microwave background; Amplitude; Intracluster medium; SIGNAL (programming language); Galaxy cluster; Dark energy; Redshift","score_opus":0.008170646269173115,"score_gpt":0.21210657551405035,"score_spread":0.20393592924487725,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2232556026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9859823,0.0000862902,0.0064654117,0.00037933272,0.00004866552,0.000029016723,0.0010171063,0.0002100075,0.005781941],"genre_scores_gemma":[0.9959441,0.000032446867,0.0026072063,0.00007412946,0.000010487206,0.00003529424,0.00068191526,0.000045616856,0.0005688637],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998178,0.00006675552,0.000006550173,0.000029338094,0.00002996648,0.000049662787],"domain_scores_gemma":[0.99780446,0.0014058787,0.00018715717,0.00010387541,0.00021684458,0.00028188885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068072556,0.00046644016,0.0005029198,0.0005280509,0.0006276076,0.00067267974,0.0011913968,0.0010519957,0.003233485],"category_scores_gemma":[0.0038044727,0.0003101912,0.0006362776,0.0005512859,0.000753853,0.0004468219,0.0008912754,0.0008919104,0.00019254485],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013037231,0.00005281249,0.010429068,0.000018280181,0.000039880095,0.0000831293,0.00004984004,0.983554,0.000619713,0.0033640778,0.00062714145,0.0010317046],"study_design_scores_gemma":[0.000052947576,0.000032020103,0.0019318517,0.0000056412973,0.000010943712,0.00001003926,0.0000319247,0.99640673,0.0003337813,0.0008986279,0.00027613444,0.000009376253],"about_ca_topic_score_codex":0.029383577,"about_ca_topic_score_gemma":0.018312661,"teacher_disagreement_score":0.029383577,"about_ca_system_score_codex":0.000828775,"about_ca_system_score_gemma":0.0007514542,"threshold_uncertainty_score":0.05842507},"labels":[],"label_agreement":null},{"id":"W2232684774","doi":"10.3847/0004-637x/817/1/49","title":"THE CHEMICAL HOMOGENEITY OF OPEN CLUSTERS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Homogeneity (statistics); Open cluster; Star cluster; Spectral line; Homogeneous; Stellar evolution; Supernova; Galaxy groups and clusters; Cluster (spacecraft)","score_opus":0.013701603138113543,"score_gpt":0.2607443908163932,"score_spread":0.24704278767827967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2232684774","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99731135,0.00009276213,0.00047860597,0.000031533527,0.0000017885297,0.0000030317879,0.00008272527,0.0000048519682,0.0019934548],"genre_scores_gemma":[0.99958974,0.000018377752,0.000113082795,0.0000066792286,0.0000029852133,0.0000017205745,0.000098122095,0.0000018696459,0.00016759493],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996315,0.000031927015,0.000013017467,0.00011636528,0.00012859645,0.00007861393],"domain_scores_gemma":[0.9980235,0.0004509332,0.00042972266,0.00014160658,0.0005781103,0.0003761167],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038396526,0.00008408051,0.0001727306,0.0013680272,0.00080489,0.0010579262,0.00039950016,0.00020704656,0.0013260323],"category_scores_gemma":[0.0027280464,0.00012761343,0.000109923945,0.0005235251,0.00079757924,0.0004095132,0.0012039371,0.00021943368,0.00017619591],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044120825,0.000033685286,0.9279314,0.000048467413,0.00011026458,0.00025647896,0.001469815,0.00810914,0.03323415,0.01102924,0.0004411056,0.01689501],"study_design_scores_gemma":[0.0000129203845,0.00007210715,0.97921354,0.000012155301,0.00002270684,0.0002250429,0.0011285278,0.005218563,0.004957644,0.0065109786,0.0026041814,0.000021646487],"about_ca_topic_score_codex":0.0057208864,"about_ca_topic_score_gemma":0.004101818,"teacher_disagreement_score":0.0057208864,"about_ca_system_score_codex":0.0008612535,"about_ca_system_score_gemma":0.00027911324,"threshold_uncertainty_score":0.011375189},"labels":[],"label_agreement":null},{"id":"W2233471020","doi":"10.1088/0004-637x/814/2/120","title":"MASS–CONCENTRATION RELATION OF CLUSTERS OF GALAXIES FROM CFHTLenS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Astrophysics; Physics; Monte Carlo method; Weak gravitational lensing; Cluster (spacecraft); Cosmology; Galaxy cluster; Galaxy; Halo; Planck; Statistical physics; Statistics; Redshift; Mathematics","score_opus":0.011492606441795101,"score_gpt":0.211027819889333,"score_spread":0.1995352134475379,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2233471020","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982377,0.00007773608,0.000464056,0.000016856604,0.0000011908309,0.0000033247177,0.0005582423,0.00003288136,0.0006079097],"genre_scores_gemma":[0.9972155,0.00002682377,0.00083869626,0.000010553994,0.0000037591285,0.0000037771251,0.0016808626,0.000011356187,0.00020847833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997452,0.00002978879,0.000010587419,0.00010239512,0.000056737234,0.00005523623],"domain_scores_gemma":[0.99857664,0.0003299294,0.0003859702,0.00025037455,0.00025120133,0.0002059843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060627615,0.00028480508,0.00027102773,0.0016947452,0.00045416478,0.00046795214,0.00040906097,0.00024676422,0.00090964773],"category_scores_gemma":[0.0018976532,0.00017251002,0.0001946245,0.00093625917,0.0003510371,0.00039769828,0.0005008524,0.00018674837,0.00017534185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019093753,0.000023717314,0.9615981,0.0000306601,0.00012578398,0.00020242188,0.0004983474,0.019922754,0.0069174827,0.0016409777,0.0012849183,0.007564019],"study_design_scores_gemma":[0.0000071008703,0.000023801174,0.9724471,0.0000049983596,0.00001863876,0.00010776218,0.000068753245,0.022838196,0.0028425516,0.00040920134,0.0012108376,0.000021063757],"about_ca_topic_score_codex":0.037178975,"about_ca_topic_score_gemma":0.03891695,"teacher_disagreement_score":0.037178975,"about_ca_system_score_codex":0.0014823194,"about_ca_system_score_gemma":0.00024851333,"threshold_uncertainty_score":0.07392514},"labels":[],"label_agreement":null},{"id":"W2235585511","doi":"10.1088/0004-637x/812/1/65","title":"FIRST<i>NuSTAR</i>OBSERVATIONS OF MRK 501 WITHIN A RADIO TO TeV MULTI-INSTRUMENT CAMPAIGN","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Foundation for Research and Technology-Hellas; Japan Society for the Promotion of Science; Jet Propulsion Laboratory; Office of Science; Instituto de Astrofísica de Canarias; Istituto Nazionale di Fisica Nucleare; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Bilim Akademisi; High Energy Accelerator Research Organization; Bulgarian Academy of Sciences; Natural Sciences and Engineering Research Council of Canada; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Crete; Smithsonian Institution; U.S. Department of Energy; Vetenskapsrådet; Max-Planck-Gesellschaft; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Hrvatska Zaklada za Znanost; European Regional Development Fund; Bundesministerium für Bildung und Forschung; Deutsche Forschungsgemeinschaft; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Russian Foundation for Basic Research; Ministry of Education, Culture, Sports, Science and Technology; California Institute of Technology; Shota Rustaveli National Science Foundation; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; Türkiye Bilimsel ve Teknolojik Araştırma Kurumu; Ministarstvo Prosvete, Nauke i Tehnološkog Razvoja; National Science Foundation; Science Foundation Ireland; Agenzia Spaziale Italiana","keywords":"Physics; Astronomy; Astrophysics","score_opus":0.03365233719160891,"score_gpt":0.23871872718453757,"score_spread":0.20506638999292867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2235585511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97763944,0.00058768713,0.0028031426,0.00018047112,0.00006518882,0.00006039909,0.008094572,0.00048245708,0.010086571],"genre_scores_gemma":[0.9527736,0.00028420534,0.0081935795,0.00035139552,0.00013379025,0.000071072136,0.034915123,0.00014697124,0.0031302252],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996278,0.000026410184,0.000025996766,0.00010474679,0.00012481686,0.00009027094],"domain_scores_gemma":[0.99917585,0.000073267634,0.00021226206,0.0001686795,0.00015394384,0.00021601282],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005659547,0.00031542158,0.00045669734,0.0010936091,0.00063326664,0.0009742726,0.0002996746,0.00044512717,0.0010522127],"category_scores_gemma":[0.0005649778,0.0002434744,0.00037939302,0.0005918615,0.0002269609,0.00037660002,0.0010874879,0.00043854676,0.00079504965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012296655,0.00042782925,0.733075,0.00029309813,0.00056760333,0.0023511443,0.001227437,0.0023169194,0.17889468,0.0010821613,0.012972302,0.06556204],"study_design_scores_gemma":[0.000015645493,0.00014071693,0.98202366,0.0000249644,0.000060120583,0.00046941024,0.00009524963,0.00068749854,0.00410997,0.000116908916,0.012230563,0.000025358087],"about_ca_topic_score_codex":0.0052533094,"about_ca_topic_score_gemma":0.022373896,"teacher_disagreement_score":0.0052533094,"about_ca_system_score_codex":0.0005081105,"about_ca_system_score_gemma":0.00035675883,"threshold_uncertainty_score":0.010445476},"labels":[],"label_agreement":null},{"id":"W2236502522","doi":"10.3847/0004-637x/818/1/77","title":"QUARK-NOVAE OCCURRING IN MASSIVE BINARIES: A UNIVERSAL ENERGY SOURCE IN SUPERLUMINOUS SUPERNOVAE WITH DOUBLE-PEAKED LIGHT CURVES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Light curve; Supernova; Astrophysics; Ejecta; Neutron star; RADIUS; Common envelope; Quark star; Accretion (finance); Magnetar; White dwarf; Strange matter; Stars","score_opus":0.008007790212431047,"score_gpt":0.20359743877156308,"score_spread":0.19558964855913202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2236502522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991916,0.000048649632,0.00041071448,0.00001317632,0.0000014631324,0.000004441246,0.00004468929,0.000013120495,0.00027235126],"genre_scores_gemma":[0.99974257,0.000009908443,0.0001205079,0.0000033045171,0.0000014480738,9.918081e-7,0.00006662705,0.0000034493298,0.00005122504],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979216,0.000042850195,0.00001571933,0.000048441943,0.00004465312,0.000056093464],"domain_scores_gemma":[0.99886155,0.00027375107,0.00035906662,0.00011727671,0.00008045879,0.00030782563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062075525,0.0005670905,0.00047809602,0.001417842,0.0006487358,0.0011615737,0.00047173142,0.00056318747,0.0011334837],"category_scores_gemma":[0.0014834548,0.00028984647,0.00048454088,0.00072262523,0.0006413323,0.00038245943,0.0011763284,0.00030079123,0.00017829426],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021811573,0.000071800896,0.9826524,0.00001340822,0.000059853315,0.00093248696,0.0000862067,0.0079043275,0.004672622,0.0010429518,0.000103951614,0.00224188],"study_design_scores_gemma":[0.000042363863,0.00017459944,0.9061627,0.000022039436,0.000042273983,0.001767741,0.00046088255,0.08441748,0.0033156418,0.0028314136,0.0007261017,0.000036761354],"about_ca_topic_score_codex":0.003670824,"about_ca_topic_score_gemma":0.0045108204,"teacher_disagreement_score":0.003670824,"about_ca_system_score_codex":0.0006428135,"about_ca_system_score_gemma":0.0002338195,"threshold_uncertainty_score":0.007298887},"labels":[],"label_agreement":null},{"id":"W2237129515","doi":"10.3847/0004-637x/820/2/82","title":"THE SCUBA-2 COSMOLOGY LEGACY SURVEY: MULTIWAVELENGTH COUNTERPARTS TO 10<sup>3</sup> SUBMILLIMETER GALAXIES IN THE UKIDSS-UDS FIELD","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Council; Leverhulme Trust; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Cosmology; Astronomy; Photometric redshift; Luminous infrared galaxy","score_opus":0.011880752447910373,"score_gpt":0.23495842582920445,"score_spread":0.22307767338129408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2237129515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99363095,0.000103932485,0.00030410205,0.000029947088,0.0000054869124,0.000012854264,0.0038792535,0.000067247805,0.0019662664],"genre_scores_gemma":[0.9882244,0.00006485482,0.0012858886,0.000037675538,0.00001881641,0.000015643314,0.009736466,0.000021184143,0.00059505604],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998604,0.000012515816,0.000011263402,0.00003418015,0.000039373692,0.00004230486],"domain_scores_gemma":[0.99863726,0.00015287782,0.0004981565,0.00021336929,0.0001997919,0.00029850693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002897343,0.00022463646,0.00014549764,0.0019992704,0.00027006224,0.00052539323,0.00038774975,0.00017774175,0.0017854142],"category_scores_gemma":[0.0007566272,0.00011768746,0.00018726081,0.0014106574,0.00018335014,0.00025267748,0.00054542266,0.0001772359,0.00085119565],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013193824,0.000034371606,0.97840184,0.000024183488,0.000033170774,0.00021898327,0.00018612912,0.00037555682,0.009146368,0.00019348663,0.001892787,0.009361178],"study_design_scores_gemma":[0.0000038601293,0.000009012921,0.9977391,0.000004284537,0.0000071795075,0.00008804586,0.000063750136,0.00040937538,0.00068155874,0.000029475445,0.00096123846,0.0000031514471],"about_ca_topic_score_codex":0.010336266,"about_ca_topic_score_gemma":0.029358495,"teacher_disagreement_score":0.010336266,"about_ca_system_score_codex":0.00023601156,"about_ca_system_score_gemma":0.00019161757,"threshold_uncertainty_score":0.020552218},"labels":[],"label_agreement":null},{"id":"W2237876737","doi":"10.3847/0004-637x/820/1/30","title":"STATISTICAL DECOUPLING OF A LAGRANGIAN FLUID PARCEL IN NEWTONIAN COSMOLOGY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Probability density function; Physics; Dynamical systems theory; Classical mechanics; Statistical physics; Decoupling (probability); Gravitational field; Gaussian; Mathematics; Quantum mechanics","score_opus":0.007584080802898882,"score_gpt":0.22618531219334972,"score_spread":0.21860123139045085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2237876737","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5601446,0.00044044934,0.41974434,0.0016126493,0.000106753294,0.000034681427,0.000108302746,0.0002924926,0.01751574],"genre_scores_gemma":[0.9793072,0.00020402706,0.017301809,0.00013386228,0.00012051104,0.000024706222,0.000054834276,0.00007564799,0.0027774207],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997658,0.00007223382,0.000008405436,0.00004380801,0.00007754791,0.000032085427],"domain_scores_gemma":[0.9991278,0.00025128367,0.00021553553,0.0001307026,0.0001422443,0.00013237426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007501481,0.0002400489,0.00042204437,0.0007258315,0.000469918,0.00086767215,0.00068044185,0.00054458866,0.0011079699],"category_scores_gemma":[0.0024752014,0.0003584874,0.00054244365,0.00029141118,0.0021829938,0.0021728415,0.0011164146,0.0009144146,0.00014464291],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000018255974,0.000021327769,0.0022916757,0.00003147924,0.000016425261,0.00012001306,0.00017923892,0.051040206,0.0027018778,0.9391911,0.0004463114,0.0039420947],"study_design_scores_gemma":[0.000010345336,0.000027118082,0.0027389233,0.000010911565,0.0000075532485,0.000083040155,0.000040286926,0.5814413,0.00070146826,0.4135981,0.0013167793,0.000024297551],"about_ca_topic_score_codex":0.004773849,"about_ca_topic_score_gemma":0.0028007193,"teacher_disagreement_score":0.004773849,"about_ca_system_score_codex":0.0010656406,"about_ca_system_score_gemma":0.0008662373,"threshold_uncertainty_score":0.009492159},"labels":[],"label_agreement":null},{"id":"W2238617295","doi":"10.3847/0004-637x/823/1/17","title":"CANDIDATE GRAVITATIONALLY LENSED DUSTY STAR-FORMING GALAXIES IN THE HERSCHEL WIDE AREA SURVEYS*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Science and Technology Facilities Council; European Commission; Gordon and Betty Moore Foundation; W. M. Keck Foundation; National Science Foundation; James S. McDonnell Foundation; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Galaxy; Redshift; Luminous infrared galaxy; Spiral galaxy; Gravitational lens; Cover (algebra); Flux (metallurgy); Spectroscopy","score_opus":0.01166807567555878,"score_gpt":0.22072016270696995,"score_spread":0.20905208703141118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2238617295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.991102,0.0005220894,0.0001609512,0.00009729355,0.0000031922784,0.0000089589785,0.0058437292,0.000051163133,0.0022106543],"genre_scores_gemma":[0.98883665,0.0002480471,0.00043974633,0.000040680614,0.000012879496,0.000006668821,0.0095275985,0.000008573542,0.00087908556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975103,0.000027076614,0.000017960307,0.000059278143,0.00006834595,0.00007634546],"domain_scores_gemma":[0.99925417,0.00012486661,0.00026586995,0.00006672635,0.0000725811,0.00021581599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003577075,0.00022941921,0.00019818381,0.00201537,0.00025718022,0.00052588125,0.00023878313,0.00016010493,0.0054684887],"category_scores_gemma":[0.0007152011,0.000089130044,0.00018946939,0.0012269217,0.00013819648,0.00032956654,0.00044556955,0.00009145013,0.0006981289],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003825042,0.000013758232,0.98813313,0.000021604894,0.000025495148,0.00006950348,0.00006669535,0.00021998773,0.001791271,0.00015392165,0.0013834425,0.008082855],"study_design_scores_gemma":[0.00000483018,0.000012764675,0.9975811,0.000007931143,0.000008757409,0.00008168041,0.000060020764,0.00028389264,0.00031817364,0.00004984773,0.0015883277,0.0000025803472],"about_ca_topic_score_codex":0.009817587,"about_ca_topic_score_gemma":0.028629884,"teacher_disagreement_score":0.009817587,"about_ca_system_score_codex":0.00038877522,"about_ca_system_score_gemma":0.00024797462,"threshold_uncertainty_score":0.019520938},"labels":[],"label_agreement":null},{"id":"W2238987790","doi":"10.3847/0004-637x/821/1/17","title":"COMPOSITIONAL SIMILARITIES AND DISTINCTIONS BETWEEN TITAN’S EVAPORITIC TERRAINS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Evaporite; Shore; Composition (language); Terrain; Feature (linguistics); Absorption (acoustics); Polar","score_opus":0.012104013684008999,"score_gpt":0.2239633812438587,"score_spread":0.2118593675598497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2238987790","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983766,0.00005573233,0.00007261424,0.000007631947,9.066381e-7,0.0000031168822,0.000061987106,0.0000056135245,0.0014157188],"genre_scores_gemma":[0.99953747,0.000025759802,0.000098633995,0.0000058392884,0.000002074236,0.0000024626665,0.00012642784,0.0000045108627,0.00019689425],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993336,0.000007924864,0.000005167821,0.000018635896,0.000014140525,0.000020703343],"domain_scores_gemma":[0.9998946,0.000017322647,0.000026147913,0.000010075362,0.000027753093,0.000024138326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000102832506,0.000087624416,0.00015034805,0.0014552362,0.0005142765,0.0005146695,0.00017857243,0.000110531146,0.0012319777],"category_scores_gemma":[0.00029924294,0.00011060717,0.00012075323,0.0007700095,0.00044019445,0.00019710399,0.000403541,0.00009116767,0.00016798942],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028494245,0.00003540298,0.89256406,0.00010406378,0.00013637778,0.0005166613,0.0035078246,0.00041536943,0.077973925,0.0006348785,0.00021104884,0.02361533],"study_design_scores_gemma":[0.0000011724086,0.000011266983,0.9988105,0.000002019718,0.0000046815685,0.0000661912,0.00038590046,0.00011958322,0.00027709588,0.000030950963,0.00028930462,0.0000013154028],"about_ca_topic_score_codex":0.010983435,"about_ca_topic_score_gemma":0.02402527,"teacher_disagreement_score":0.010983435,"about_ca_system_score_codex":0.00027946182,"about_ca_system_score_gemma":0.0001666574,"threshold_uncertainty_score":0.021839023},"labels":[],"label_agreement":null},{"id":"W2239221342","doi":"10.3847/0004-637x/818/1/63","title":"DISCOVERY OF X-RAY EMISSION FROM THE GALACTIC SUPERNOVA REMNANT G32.8-0.1 WITH SUZAKU","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Supernova remnant; Ionization; Near-Earth supernova; Spectral index; Emission spectrum; Molecular cloud; Supergiant; Spectral line","score_opus":0.007567707442954735,"score_gpt":0.20532556427328297,"score_spread":0.19775785683032823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2239221342","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99734676,0.0004059199,0.00040400974,0.00003728216,0.00001012487,0.000013143215,0.00038625914,0.000069044785,0.0013274684],"genre_scores_gemma":[0.9931652,0.00018678315,0.0030059868,0.00007013827,0.000023771941,0.000025113466,0.0024393108,0.00005362027,0.001030013],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998919,0.000009384754,0.000007971904,0.000030297679,0.000028869857,0.000031584987],"domain_scores_gemma":[0.99955684,0.000026284664,0.00010886859,0.00009009253,0.000065777844,0.0001520508],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034894224,0.00074674987,0.00038195675,0.00090035575,0.00054425374,0.0004413726,0.0005534181,0.00045741684,0.0014016296],"category_scores_gemma":[0.0003534708,0.00034396487,0.0004236874,0.00053372514,0.00024794365,0.00031049325,0.001070256,0.0003840392,0.00078840717],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007596178,0.00011372918,0.22368756,0.0002262875,0.00025473483,0.005289153,0.00066015305,0.00033254465,0.75441235,0.0002886805,0.0008404178,0.013134855],"study_design_scores_gemma":[0.00002692297,0.00041759346,0.9578654,0.000025123654,0.00013717868,0.0036458927,0.00026383874,0.0007300497,0.028007345,0.00014160597,0.00871797,0.000021033964],"about_ca_topic_score_codex":0.0012910062,"about_ca_topic_score_gemma":0.0031179711,"teacher_disagreement_score":0.0014016296,"about_ca_system_score_codex":0.00019655637,"about_ca_system_score_gemma":0.000115693954,"threshold_uncertainty_score":0.0046889186},"labels":[],"label_agreement":null},{"id":"W2239547061","doi":"10.3847/0004-637x/819/2/131","title":"He II λ4686 EMISSION FROM THE MASSIVE BINARY SYSTEM IN η CAR: CONSTRAINTS TO THE ORBITAL ELEMENTS AND THE NATURE OF THE PERIODIC MINIMA*†‡§","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministério da Ciência, Tecnologia e Inovação; Ciência sem Fronteiras; Consejo Nacional de Investigaciones Científicas y Técnicas; Western Michigan University; Michigan State University; College of Engineering, Michigan State University; National Aeronautics and Space Administration; Space Telescope Science Institute; University of North Carolina at Chapel Hill; National Science Foundation","keywords":"Physics; Astrophysics; Orbital inclination; Emission spectrum; Orbital elements; Line (geometry); Binary number; Longitude; Spectral line; Astronomy; Geometry; Latitude","score_opus":0.005213504485554835,"score_gpt":0.20931801059807892,"score_spread":0.2041045061125241,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2239547061","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99950874,0.000023395272,0.00009865073,0.000008645931,0.00000111229,9.692031e-7,0.000030603587,0.0000021336557,0.00032576403],"genre_scores_gemma":[0.99983394,0.000009137908,0.000045844576,0.0000022258503,0.0000012215127,4.8759006e-7,0.000044342778,6.351215e-7,0.00006214636],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999465,0.0000056892004,0.0000034654888,0.00002047961,0.000011028983,0.000012780771],"domain_scores_gemma":[0.99986017,0.000018581508,0.000053031814,0.000012587538,0.00002441224,0.000031126063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018202403,0.000117613075,0.00013410802,0.00028429343,0.000505559,0.0004291015,0.00024324583,0.00020959413,0.00080297794],"category_scores_gemma":[0.00027520195,0.00011468464,0.00012698708,0.00020740833,0.0001973511,0.00017155077,0.00027215644,0.00015306361,0.00018888117],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016631659,0.000057144625,0.9652547,0.000014063448,0.00002275277,0.00021751516,0.00014474402,0.001225698,0.0283213,0.0002720099,0.00012710581,0.0041765505],"study_design_scores_gemma":[0.0000029225082,0.000027608114,0.99399513,0.000002703105,0.0000073960437,0.00010980717,0.00012423657,0.0042271544,0.0011774272,0.00007906143,0.00024268522,0.0000039769393],"about_ca_topic_score_codex":0.0073455907,"about_ca_topic_score_gemma":0.011185006,"teacher_disagreement_score":0.0073455907,"about_ca_system_score_codex":0.00034381813,"about_ca_system_score_gemma":0.00013412925,"threshold_uncertainty_score":0.014605641},"labels":[],"label_agreement":null},{"id":"W2244461708","doi":"10.3847/0004-637x/831/1/80","title":"NuSTAR OBSERVATIONS OF MAGNETAR 1E 1048.1–5937","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Black-body radiation; Photon; Gamma ray; Neutron star; Nuclear physics; Radiation; Optics","score_opus":0.021847797920990647,"score_gpt":0.3008018592124522,"score_spread":0.2789540612914616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2244461708","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99469286,0.00026924865,0.0003239339,0.0000333712,0.000010151913,0.000006307748,0.0010077481,0.00009932451,0.0035569258],"genre_scores_gemma":[0.9948974,0.00008692507,0.0013437629,0.00003827489,0.000014337693,0.000007705317,0.0028117083,0.000017908123,0.00078188966],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998349,0.000011940172,0.000008669016,0.00005023775,0.00006239418,0.000031869895],"domain_scores_gemma":[0.9997378,0.000022837901,0.0000835214,0.000035320663,0.000058981313,0.000061537794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024368921,0.00017423788,0.00037760823,0.0009775963,0.0003043123,0.00030498873,0.00031522766,0.00026488584,0.001288874],"category_scores_gemma":[0.0003786229,0.00013210431,0.00015085224,0.0005297392,0.00012498353,0.00018496349,0.00033661054,0.00017964099,0.0006743027],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009707395,0.00019978464,0.627267,0.00017420374,0.00022925591,0.001180333,0.00047610214,0.0020402009,0.31383374,0.00073471153,0.004731514,0.048162453],"study_design_scores_gemma":[0.000030707008,0.00023040034,0.9852594,0.000018478111,0.000037736707,0.00074385206,0.000079925194,0.0014754118,0.006500271,0.00012135907,0.0054860013,0.000016469463],"about_ca_topic_score_codex":0.003115651,"about_ca_topic_score_gemma":0.010977294,"teacher_disagreement_score":0.003115651,"about_ca_system_score_codex":0.00043957887,"about_ca_system_score_gemma":0.00012860131,"threshold_uncertainty_score":0.0061950088},"labels":[],"label_agreement":null},{"id":"W2244785912","doi":"10.1088/0004-637x/736/2/90","title":"PROBING THE GC-LMXB CONNECTION IN NGC 1399: A WIDE-FIELD STUDY WITH THE<i>HUBBLE SPACE TELESCOPE</i>AND<i>CHANDRA</i>","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Elliptical galaxy; Galaxy; Astronomy; Metallicity; Dwarf galaxy","score_opus":0.009418508515428772,"score_gpt":0.19944648936728598,"score_spread":0.1900279808518572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2244785912","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992349,0.000077410186,0.00008952359,0.000009411256,0.0000010586754,0.0000027604992,0.00021098032,0.0000056305644,0.00036833223],"genre_scores_gemma":[0.998478,0.000098584715,0.00045251223,0.000011028383,0.000008909338,0.000003416844,0.0007294177,0.0000056164617,0.00021246061],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998981,0.000008538273,0.0000049908995,0.00004097167,0.00002031559,0.000027167329],"domain_scores_gemma":[0.9996468,0.00003447426,0.00010734158,0.00003690557,0.000041093077,0.00013334272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020690644,0.00026326894,0.00022002238,0.0011043093,0.0005696174,0.0004222683,0.00029585723,0.00021143391,0.000835335],"category_scores_gemma":[0.0002591239,0.00012891796,0.00021114945,0.0010129219,0.0003076052,0.00040312647,0.00057917734,0.00020555005,0.00022971732],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015535283,0.00010756133,0.9635451,0.000023971174,0.00007653297,0.0005058887,0.00037050174,0.00028137822,0.027271561,0.0001417968,0.00020715006,0.0073131947],"study_design_scores_gemma":[0.000002212369,0.000021124297,0.9987816,0.0000022634217,0.0000114081,0.0001777097,0.00011011866,0.0001754453,0.00040378442,0.000028395776,0.00028300466,0.0000028253432],"about_ca_topic_score_codex":0.011773348,"about_ca_topic_score_gemma":0.020150304,"teacher_disagreement_score":0.011773348,"about_ca_system_score_codex":0.0003266207,"about_ca_system_score_gemma":0.00016819281,"threshold_uncertainty_score":0.023409665},"labels":[],"label_agreement":null},{"id":"W2245211555","doi":"10.3847/0004-637x/818/1/97","title":"RESOLVED CO GAS INTERIOR TO THE DUST RINGS OF THE HD 141569 DISK","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Academia Sinica; California Institute of Technology; Smithsonian Astrophysical Observatory; Gordon and Betty Moore Foundation; National Science Foundation; James S. McDonnell Foundation; Smithsonian Institution","keywords":"Debris; Physics; RADIUS; Debris disk; Black-body radiation; Astrophysics; Excitation; Infrared; Astronomy; Optics; Stars; Planetary system; Meteorology","score_opus":0.010195412386982043,"score_gpt":0.2400136028306675,"score_spread":0.22981819044368546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2245211555","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988531,0.00007958964,0.00016275802,0.000009743898,0.0000027779222,0.0000015924538,0.00012428363,0.000011465887,0.00075463054],"genre_scores_gemma":[0.9996055,0.00001769578,0.0001609744,0.0000059637805,0.000003070746,0.0000014128118,0.0000910533,0.0000017554647,0.00011263833],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999392,0.0000032852902,0.000003290539,0.000025756197,0.000011444274,0.000017011635],"domain_scores_gemma":[0.9998616,0.000021368704,0.000050359256,0.000017726736,0.000015588315,0.00003319607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007093716,0.00011570973,0.00021545419,0.00039411135,0.00029301475,0.0004712914,0.0001625796,0.00015627072,0.0008763611],"category_scores_gemma":[0.00022485972,0.00014438784,0.00012352478,0.00021355154,0.00022320154,0.00015631916,0.00041175188,0.00015523854,0.00015687806],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055130845,0.00005764234,0.33090872,0.000058593978,0.00007279708,0.0010133341,0.00039043828,0.00083748344,0.6566723,0.0004257407,0.00027918324,0.0087324465],"study_design_scores_gemma":[0.000010832633,0.00003283139,0.98181665,0.0000048497473,0.000016106764,0.0003414685,0.00017755576,0.00090219366,0.015969384,0.00009284488,0.0006300502,0.000005269997],"about_ca_topic_score_codex":0.0015163746,"about_ca_topic_score_gemma":0.001671998,"teacher_disagreement_score":0.0015163746,"about_ca_system_score_codex":0.0002534776,"about_ca_system_score_gemma":0.000069889895,"threshold_uncertainty_score":0.0030151606},"labels":[],"label_agreement":null},{"id":"W2246618421","doi":"10.1088/0004-637x/772/2/121","title":"LENSING NOISE IN MILLIMETER-WAVE GALAXY CLUSTER SURVEYS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Cosmic microwave background; Galaxy cluster; Gravitational lens; Galaxy; Sunyaev–Zel'dovich effect; Weak gravitational lensing; Cluster (spacecraft); Cosmic variance; South Pole Telescope; Astronomy; Redshift","score_opus":0.012812218328787095,"score_gpt":0.20930707033653564,"score_spread":0.19649485200774855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2246618421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96608126,0.0009467185,0.029185973,0.00039562583,0.000024924708,0.000029650351,0.000664239,0.00027151866,0.002400171],"genre_scores_gemma":[0.996335,0.00019637332,0.0024967566,0.00005738716,0.00003431846,0.00001102526,0.00058441807,0.000025416144,0.0002592736],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9983354,0.0006943733,0.00007473642,0.00033272477,0.00041462027,0.0001480994],"domain_scores_gemma":[0.9832485,0.012015314,0.002607014,0.0010346405,0.0008002913,0.0002942573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029232537,0.00030931263,0.00034724383,0.0012463126,0.00026885374,0.0008055895,0.00049847696,0.00056201336,0.0004538476],"category_scores_gemma":[0.025915688,0.0002638811,0.00022595127,0.0018312408,0.00034426732,0.00080856844,0.00051099557,0.00029148703,0.00016616075],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029409648,0.000038009868,0.8504083,0.00014600453,0.00019093826,0.00024418256,0.0002960244,0.09587612,0.0071655684,0.011922835,0.0014863241,0.03193168],"study_design_scores_gemma":[0.000031927,0.00009131041,0.8333206,0.00005801746,0.00006425831,0.00027275775,0.00016223366,0.15130813,0.0043284246,0.0079375105,0.0023802577,0.000044531876],"about_ca_topic_score_codex":0.0074813846,"about_ca_topic_score_gemma":0.0053554974,"teacher_disagreement_score":0.0074813846,"about_ca_system_score_codex":0.00097147096,"about_ca_system_score_gemma":0.00027463422,"threshold_uncertainty_score":0.0154598355},"labels":[],"label_agreement":null},{"id":"W2246786832","doi":"10.3847/0004-637x/822/1/32","title":"A HUBBLE SPACE TELESCOPE STUDY OF THE ENIGMATIC MILKY WAY HALO GLOBULAR CLUSTER CRATER*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Globular cluster; Astrophysics; Milky Way; Astronomy; Impact crater; Blue straggler; Dwarf galaxy; Star cluster; Stellar population; Horizontal branch; Galaxy; Metallicity; Population; Red-giant branch; Star formation","score_opus":0.00905775651414082,"score_gpt":0.21741408749792018,"score_spread":0.20835633098377937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2246786832","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963737,0.000044364508,0.00001782283,0.00002776051,5.070985e-7,0.0000015468027,0.00007954775,0.0000014123316,0.00018966741],"genre_scores_gemma":[0.99947983,0.000045050074,0.00004844871,0.000013165021,0.0000029637333,6.9260454e-7,0.00013860861,0.0000013517632,0.000269894],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994946,0.0000052820283,0.0000017115167,0.000014738958,0.000008359291,0.000020567553],"domain_scores_gemma":[0.9997447,0.00003450066,0.00006448387,0.000021979491,0.00003054313,0.00010378076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018673786,0.00015106153,0.00010843662,0.0009788255,0.0005083527,0.00040379417,0.000285592,0.0002613425,0.0010717986],"category_scores_gemma":[0.0004393849,0.00010691234,0.00018089627,0.0005642231,0.00032536575,0.00025946827,0.00030432883,0.00020612097,0.00018159427],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050167844,0.000027370319,0.9926455,0.000008098664,0.000026365718,0.00058242824,0.0010207011,0.0002224541,0.0017186888,0.0002395034,0.00032740633,0.0031312758],"study_design_scores_gemma":[8.0340726e-7,0.000009333016,0.9989066,0.0000030860845,0.000003796785,0.000108051936,0.00043424772,0.00022043035,0.000057955625,0.000021845843,0.00023220154,0.0000016831141],"about_ca_topic_score_codex":0.118977435,"about_ca_topic_score_gemma":0.20408514,"teacher_disagreement_score":0.118977435,"about_ca_system_score_codex":0.0010233062,"about_ca_system_score_gemma":0.00031536174,"threshold_uncertainty_score":0.23656982},"labels":[],"label_agreement":null},{"id":"W2246800589","doi":"10.3847/0004-637x/818/2/118","title":"PRINCIPAL COMPONENT ANALYSIS STUDIES OF TURBULENCE IN OPTICALLY THICK GAS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Principal component analysis; Spectral density; Fractional Brownian motion; Turbulence; Radiative transfer; Spectral line; Noise (video); Fourier transform","score_opus":0.02061476706432522,"score_gpt":0.2799760182152579,"score_spread":0.25936125115093267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2246800589","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9365645,0.00023034614,0.06179782,0.00010563912,0.000026023725,0.000025456115,0.00018280259,0.00015013973,0.0009172981],"genre_scores_gemma":[0.99020946,0.00009504078,0.009301633,0.0000051578863,0.00001403367,0.000010919692,0.00017646616,0.000020610109,0.00016664928],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99974364,0.00010179926,0.000015276888,0.00003501994,0.00007239428,0.00003188629],"domain_scores_gemma":[0.9977883,0.0014198527,0.00025746832,0.00016138867,0.0002907227,0.000082177314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081065187,0.00031252642,0.00019254394,0.001268678,0.00030916432,0.0007313197,0.00015325563,0.00015193853,0.00052946457],"category_scores_gemma":[0.0034577635,0.00011467873,0.00034294752,0.00097319414,0.0004245255,0.0003521785,0.00032344356,0.00029981864,0.0000845607],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008375884,0.0003236981,0.17848763,0.0003059699,0.0005419173,0.00079416233,0.0014977606,0.40318054,0.14346376,0.031383727,0.0028169656,0.23636633],"study_design_scores_gemma":[0.000012247229,0.00014236433,0.20785454,0.000023525188,0.00003796134,0.00013417301,0.00024038294,0.7735021,0.009825908,0.0070466488,0.0011348613,0.000045274042],"about_ca_topic_score_codex":0.0021737826,"about_ca_topic_score_gemma":0.000996106,"teacher_disagreement_score":0.0021737826,"about_ca_system_score_codex":0.0001838035,"about_ca_system_score_gemma":0.00021392468,"threshold_uncertainty_score":0.004322231},"labels":[],"label_agreement":null},{"id":"W2247847363","doi":"10.1088/0004-637x/807/2/166","title":"PROSPECTS FOR DELENSING THE COSMIC MICROWAVE BACKGROUND FOR STUDYING INFLATION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cosmic microwave background; Physics; Gravitational lens; Astrophysics; Polarization (electrochemistry); Gravitational wave; Cosmic infrared background; Inflation (cosmology); Anisotropy; Astronomy; Optics; Galaxy; Redshift","score_opus":0.037796054530567495,"score_gpt":0.29083386395029787,"score_spread":0.25303780941973036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2247847363","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7448837,0.020554714,0.18898962,0.015392098,0.0003917196,0.00009796989,0.002321142,0.0015852267,0.025783839],"genre_scores_gemma":[0.89576536,0.004225559,0.095282696,0.0011861774,0.00038995707,0.0001176727,0.0014672052,0.0001600631,0.0014053397],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994437,0.00024352844,0.00001506435,0.00012984814,0.00009834897,0.00006955376],"domain_scores_gemma":[0.99612916,0.001341705,0.00054239976,0.000853882,0.0003568585,0.0007759566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0048547005,0.0009864612,0.00067420176,0.0009989748,0.00046627413,0.0014072962,0.0010656569,0.0012135556,0.0017111169],"category_scores_gemma":[0.005400175,0.0005980241,0.00039699694,0.0009887716,0.0011088046,0.0026357898,0.0016627437,0.0021470156,0.0006009827],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017523228,0.00027851734,0.3913959,0.0007998479,0.00047249568,0.00066675665,0.0009619993,0.020028265,0.18464305,0.17320158,0.0050065205,0.22079274],"study_design_scores_gemma":[0.00017336145,0.0007468726,0.52138406,0.00033917348,0.00036176344,0.00084365025,0.00076463964,0.071069956,0.06327653,0.27995744,0.060683426,0.00039908302],"about_ca_topic_score_codex":0.0009569415,"about_ca_topic_score_gemma":0.0012556124,"teacher_disagreement_score":0.0048547005,"about_ca_system_score_codex":0.00064747414,"about_ca_system_score_gemma":0.000409586,"threshold_uncertainty_score":0.025674403},"labels":[],"label_agreement":null},{"id":"W2252322915","doi":"10.3847/0004-637x/824/2/134","title":"BALLOON-BORNE SUBMILLIMETER POLARIMETRY OF THE VELA C MOLECULAR CLOUD: SYSTEMATIC DEPENDENCE OF POLARIZATION FRACTION ON COLUMN DENSITY AND LOCAL POLARIZATION-ANGLE DISPERSION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Polarization (electrochemistry); Vela; Polarimetry; Molecular cloud; Polarimeter; Magnetic field; Telescope; Green Bank Telescope; Population","score_opus":0.004982206797617629,"score_gpt":0.20624093258481285,"score_spread":0.20125872578719523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2252322915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99786526,0.000054979257,0.00055741775,0.000019253466,0.0000031912407,0.0000053295016,0.00079917297,0.00003617224,0.0006591979],"genre_scores_gemma":[0.99857986,0.000022911632,0.0003439227,0.000009335553,0.0000040448954,0.000005164942,0.0009396452,0.000012957671,0.000082159095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984026,0.000023983392,0.0000056973595,0.000046448127,0.00004739623,0.00003613984],"domain_scores_gemma":[0.9994241,0.00013109246,0.00014814614,0.00013182599,0.00010097342,0.000063934225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003664318,0.00018611393,0.00016325506,0.0007153623,0.00048136423,0.0004343559,0.00027509205,0.0002320386,0.0004098469],"category_scores_gemma":[0.000858316,0.00018949612,0.00022225842,0.00064213877,0.00022291676,0.00019016348,0.00030472627,0.00022378413,0.00012435703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026110213,0.00006621381,0.91036457,0.000027311218,0.0001787761,0.000090513386,0.00017016316,0.004128093,0.0758776,0.00017797555,0.000559774,0.008097864],"study_design_scores_gemma":[0.0000050341996,0.000011024841,0.99367815,0.0000030135755,0.000012267541,0.000026691583,0.00002606805,0.0033832365,0.0025873133,0.000026032772,0.00023523798,0.000005903086],"about_ca_topic_score_codex":0.015240977,"about_ca_topic_score_gemma":0.021357201,"teacher_disagreement_score":0.015240977,"about_ca_system_score_codex":0.00033984942,"about_ca_system_score_gemma":0.00018753849,"threshold_uncertainty_score":0.030304492},"labels":[],"label_agreement":null},{"id":"W2253571065","doi":"10.3847/0004-637x/818/2/175","title":"FORMING THE COLD CLASSICAL KUIPER BELT IN A LIGHT DISK","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Solar System; Nice model; Formation and evolution of the Solar System; Solar mass; Asteroid belt","score_opus":0.0066354216113797045,"score_gpt":0.20435916075001104,"score_spread":0.19772373913863134,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2253571065","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954846,0.00007344177,0.0014505086,0.00006707375,0.000004110681,0.000007546976,0.000019538495,0.000019702256,0.0028734165],"genre_scores_gemma":[0.99890697,0.000021253009,0.00050840527,0.000023393855,0.000005685428,0.0000029870118,0.000028743667,0.0000027903682,0.0004997152],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999317,0.000007001458,0.0000025237648,0.00002377155,0.000012716886,0.000022241806],"domain_scores_gemma":[0.9997143,0.000026613,0.00008518824,0.000037528916,0.0000151966515,0.00012107448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017693805,0.0002126439,0.00024696594,0.000433861,0.0007895285,0.0012604005,0.0010440815,0.0005992782,0.0018994722],"category_scores_gemma":[0.0004125782,0.0001942602,0.00023682011,0.0002359857,0.0012413315,0.00084031624,0.0010326959,0.0002523231,0.00035349926],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012951862,0.00043993475,0.6607735,0.00020685878,0.00017744771,0.006471536,0.0031601305,0.0365616,0.166364,0.09881604,0.0020079818,0.023725778],"study_design_scores_gemma":[0.00044825362,0.0010619654,0.6532626,0.000055580473,0.00014733041,0.0052042017,0.004776145,0.21941106,0.018648054,0.08018418,0.016648434,0.00015217428],"about_ca_topic_score_codex":0.0028845929,"about_ca_topic_score_gemma":0.0027799876,"teacher_disagreement_score":0.0028845929,"about_ca_system_score_codex":0.0008870401,"about_ca_system_score_gemma":0.00018436604,"threshold_uncertainty_score":0.0064359307},"labels":[],"label_agreement":null},{"id":"W2253985754","doi":"10.3847/0004-637x/819/2/143","title":"CONTRACTION SIGNATURES TOWARD DENSE CORES IN THE PERSEUS MOLECULAR CLOUD","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Contraction (grammar); Asymmetry; Dimensionless quantity; Molecular cloud; Supersonic speed; James Clerk Maxwell Telescope; Spectral line; Emission spectrum","score_opus":0.009701349999329291,"score_gpt":0.2411364710416226,"score_spread":0.23143512104229333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2253985754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996884,0.000021833832,0.000032955813,0.0000030550282,2.9019898e-7,0.0000013556528,0.000045359728,0.0000032786545,0.00020359125],"genre_scores_gemma":[0.999765,0.00001742079,0.000070759525,0.0000039556735,0.0000011921184,9.116905e-7,0.00008417386,8.800128e-7,0.000055758384],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999486,0.0000059697886,0.000002426173,0.000015158046,0.000015392638,0.000012490137],"domain_scores_gemma":[0.9997501,0.00003208915,0.00009550676,0.000018098064,0.000044349836,0.000059913156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016464072,0.00021913095,0.000118402226,0.0008784897,0.00020829498,0.000215507,0.0001559489,0.000079218,0.00043349472],"category_scores_gemma":[0.0003078954,0.00008762557,0.000063733765,0.00032371568,0.00022674871,0.00012106383,0.00030193906,0.00006819046,0.00010382391],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011385805,0.000017614266,0.9692969,0.000009779144,0.000021263888,0.00023974452,0.00020472005,0.0006774798,0.024249664,0.000091272435,0.000082714374,0.00499493],"study_design_scores_gemma":[0.0000072037933,0.000032675453,0.9965989,0.0000025582508,0.0000052297323,0.00013777282,0.000104167004,0.0007455219,0.0020893232,0.000035281526,0.00023945494,0.0000018717418],"about_ca_topic_score_codex":0.011062009,"about_ca_topic_score_gemma":0.014076189,"teacher_disagreement_score":0.011062009,"about_ca_system_score_codex":0.0002971848,"about_ca_system_score_gemma":0.00013792937,"threshold_uncertainty_score":0.021995187},"labels":[],"label_agreement":null},{"id":"W2256577165","doi":"10.3847/0004-637x/817/1/58","title":"GLOBULAR CLUSTER SYSTEMS IN BRIGHTEST CLUSTER GALAXIES. II. NGC 6166","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Metallicity; Galaxy; Advanced Camera for Surveys; RADIUS; Halo; Photometry (optics); Intracluster medium; Astronomy; Hubble space telescope; Galaxy cluster; Stars; Computer science","score_opus":0.0061635182768985915,"score_gpt":0.20105200051074115,"score_spread":0.19488848223384256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2256577165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99739033,0.00032756102,0.000043193933,0.00004180252,0.0000065877302,0.000002583032,0.00051268167,0.000013196139,0.0016621688],"genre_scores_gemma":[0.99791604,0.00011761922,0.000116682866,0.000022586788,0.000009978658,0.0000022846984,0.00096896046,0.0000028155414,0.0008430803],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985635,0.000007812993,0.000010254639,0.000037964994,0.000032891672,0.000054719814],"domain_scores_gemma":[0.99960345,0.000018531404,0.00015994361,0.000030716317,0.00004689002,0.00014058602],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013184684,0.00025450584,0.00021069996,0.0019202771,0.00072624977,0.00060888554,0.00019343013,0.00025664014,0.004807838],"category_scores_gemma":[0.0003874798,0.000119615914,0.00015923225,0.0013735677,0.00033526414,0.00045706166,0.00085259875,0.00021636512,0.0007272429],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009903564,0.000025612462,0.98447025,0.000026752796,0.000013285556,0.0002868647,0.0004035409,0.00015821202,0.004714219,0.00027701928,0.0005264837,0.008998622],"study_design_scores_gemma":[0.0000018608282,0.00001227319,0.998776,0.00000418249,0.0000031653153,0.00019480273,0.00011472248,0.000048865048,0.00009712787,0.0000831776,0.00066197343,0.0000017910284],"about_ca_topic_score_codex":0.017354518,"about_ca_topic_score_gemma":0.029400289,"teacher_disagreement_score":0.017354518,"about_ca_system_score_codex":0.00042478394,"about_ca_system_score_gemma":0.0001545463,"threshold_uncertainty_score":0.034507036},"labels":[],"label_agreement":null},{"id":"W2256921252","doi":"10.3847/0004-637x/820/1/38","title":"DISPERSION OF MAGNETIC FIELDS IN MOLECULAR CLOUDS. IV. ANALYSIS OF INTERFEROMETRY DATA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Algorithm; Computer science","score_opus":0.012082605771853513,"score_gpt":0.2523992791196523,"score_spread":0.2403166733477988,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2256921252","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95797,0.00012969083,0.040251333,0.00010162759,0.000012245091,0.000012262643,0.0003640162,0.00024462267,0.0009142712],"genre_scores_gemma":[0.9943901,0.000036754303,0.005195952,0.000006419458,0.000011173079,0.0000030433405,0.00021100196,0.000014723281,0.00013082782],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998952,0.000014682716,0.000007877972,0.000023191555,0.000034956705,0.000024077966],"domain_scores_gemma":[0.9995814,0.000094186726,0.00012322504,0.00010557943,0.000064867316,0.00003076988],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000343908,0.0001782147,0.00013864075,0.0014722422,0.00029364874,0.00041979176,0.00023573628,0.000190385,0.0003302245],"category_scores_gemma":[0.0014305939,0.00011843622,0.0002396247,0.0007725065,0.0003017848,0.0004113706,0.00027380468,0.00033128716,0.000094759074],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034264755,0.00015228895,0.3807635,0.00011917284,0.00022682571,0.00042175516,0.0006975509,0.1962639,0.24406154,0.024016611,0.0015999116,0.15133435],"study_design_scores_gemma":[0.000019248842,0.000047730522,0.41985857,0.000013704804,0.000022926966,0.00021071045,0.00008743777,0.550129,0.020160202,0.007585859,0.001808553,0.000056118948],"about_ca_topic_score_codex":0.006089089,"about_ca_topic_score_gemma":0.003747307,"teacher_disagreement_score":0.006089089,"about_ca_system_score_codex":0.00036881177,"about_ca_system_score_gemma":0.00023162301,"threshold_uncertainty_score":0.012107313},"labels":[],"label_agreement":null},{"id":"W2257435077","doi":"10.1088/0004-637x/814/1/3","title":"THE PANCHROMATIC HUBBLE ANDROMEDA TREASURY. VIII. A WIDE-AREA, HIGH-RESOLUTION MAP OF DUST EXTINCTION IN M31","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Extinction (optical mineralogy); Panchromatic film; Andromeda; Milky Way; Red-giant branch; Galaxy; Circumstellar dust; Population; Dust lane","score_opus":0.011871339137772293,"score_gpt":0.20900010519238052,"score_spread":0.19712876605460822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2257435077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9037141,0.001649581,0.0061572455,0.0008257212,0.0000613508,0.00011490118,0.050024346,0.0014299173,0.036022924],"genre_scores_gemma":[0.9614198,0.00045617242,0.014483898,0.000091779206,0.00004956219,0.0000400599,0.016358698,0.000188141,0.0069119106],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998604,0.000011516417,0.0000033013785,0.000043543532,0.000052432188,0.000028783123],"domain_scores_gemma":[0.999691,0.000013273079,0.00010801208,0.00006136789,0.000059674738,0.000066705245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012830955,0.00030900785,0.0001357299,0.001355319,0.0003016893,0.0004150896,0.0002782296,0.00021534327,0.0033891455],"category_scores_gemma":[0.00038093657,0.00014160498,0.00027053358,0.0009693754,0.000104218,0.00032033463,0.0003540456,0.0002768792,0.001370973],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034082253,0.00006783229,0.65769154,0.00020784292,0.00034920286,0.0008214548,0.0007866857,0.0040267915,0.08665286,0.002539823,0.05754676,0.18896839],"study_design_scores_gemma":[0.000009172978,0.000013868721,0.97784585,0.000011410558,0.000011339417,0.00021849474,0.000045127264,0.0015819323,0.0014696474,0.00020233607,0.01858198,0.000008740822],"about_ca_topic_score_codex":0.07092746,"about_ca_topic_score_gemma":0.12023832,"teacher_disagreement_score":0.07092746,"about_ca_system_score_codex":0.00052719994,"about_ca_system_score_gemma":0.00034039104,"threshold_uncertainty_score":0.14102924},"labels":[],"label_agreement":null},{"id":"W2257764839","doi":"10.3847/0004-637x/822/2/91","title":"METAL DIFFUSION IN SMOOTHED PARTICLE HYDRODYNAMICS SIMULATIONS OF DWARF GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council","keywords":"Metallicity; Smoothed-particle hydrodynamics; Diffusion; Galaxy; Outflow; Dwarf galaxy; Stars","score_opus":0.007425047811045637,"score_gpt":0.21640232548265115,"score_spread":0.2089772776716055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2257764839","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98840964,0.00013221889,0.0066130296,0.0003641612,0.000068159185,0.000051648552,0.00035410534,0.00026450527,0.003742517],"genre_scores_gemma":[0.99423176,0.00006245998,0.003978197,0.00010685362,0.000027673423,0.000056629837,0.00049651123,0.00006848801,0.000971486],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99965584,0.00009971553,0.000016894064,0.00004414144,0.00006724568,0.000116135176],"domain_scores_gemma":[0.9969516,0.0015956137,0.0002572166,0.00017661233,0.00044347692,0.00057539897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010808484,0.0007116897,0.0012519534,0.0010627604,0.0010514811,0.0012424842,0.0019054943,0.0017611973,0.0017988716],"category_scores_gemma":[0.0045127817,0.0006768274,0.0013403452,0.0008402935,0.0019824859,0.00075783185,0.00095630484,0.0014920769,0.00019451746],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021250815,0.00015142065,0.008165389,0.000028293674,0.00009136681,0.00014770255,0.00010787275,0.9859072,0.0012617756,0.0026636922,0.00039002416,0.0008728032],"study_design_scores_gemma":[0.00006309253,0.000033347453,0.0012012155,0.0000048565,0.000011345618,0.000006580752,0.00003038429,0.9976927,0.00026299033,0.0005286261,0.00015342199,0.00001155812],"about_ca_topic_score_codex":0.061763275,"about_ca_topic_score_gemma":0.018841946,"teacher_disagreement_score":0.061763275,"about_ca_system_score_codex":0.0024390833,"about_ca_system_score_gemma":0.0019638808,"threshold_uncertainty_score":0.12280756},"labels":[],"label_agreement":null},{"id":"W2258245628","doi":"10.3847/0004-637x/819/1/65","title":"POLYCYCLIC AROMATIC HYDROCARBON EMISSION IN SPITZER/IRS MAPS. I. CATALOG AND SIMPLE DIAGNOSTICS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Reflection nebula; Physics; Astrophysics; Molecular cloud; Nebula; Infrared; Spectrograph; Interstellar medium; Spectral resolution; Spectral line; Astronomy; Galaxy; Stars","score_opus":0.0069782707466085276,"score_gpt":0.22573543416818978,"score_spread":0.21875716342158125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2258245628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98742,0.00028344506,0.0009378945,0.000019873773,0.0000030085823,0.00004093688,0.008069519,0.00017240216,0.003052924],"genre_scores_gemma":[0.97518003,0.00024183604,0.0032294982,0.000016914279,0.00001970123,0.000044888202,0.020147039,0.000056191115,0.0010639126],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960405,0.000027307091,0.000052919222,0.000088697845,0.0001553719,0.000071643284],"domain_scores_gemma":[0.9988343,0.00013554005,0.000388293,0.00028854358,0.00026404817,0.000089267196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004210239,0.00032889235,0.00021174883,0.005817014,0.00025570954,0.0007311511,0.00037950266,0.00023855898,0.0022844155],"category_scores_gemma":[0.0009937817,0.00015007204,0.00026255578,0.003580454,0.0003124305,0.00055746525,0.00071576255,0.00014254707,0.0012682714],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013065757,0.000053210108,0.95900047,0.0000731646,0.000044237597,0.00015005717,0.00019443932,0.0009222778,0.0091598295,0.00031404998,0.00090472575,0.029052919],"study_design_scores_gemma":[0.000002704792,0.000022370468,0.9966037,0.000006132555,0.000011582095,0.00012419277,0.00006960864,0.000557735,0.0011765598,0.000055952394,0.001365765,0.0000035629207],"about_ca_topic_score_codex":0.0054210396,"about_ca_topic_score_gemma":0.0074024536,"teacher_disagreement_score":0.005817014,"about_ca_system_score_codex":0.00023539289,"about_ca_system_score_gemma":0.00018321733,"threshold_uncertainty_score":0.010778964},"labels":[],"label_agreement":null},{"id":"W2258780167","doi":"10.3847/1538-4357/833/2/169","title":"RESOLVING MICROLENSING EVENTS WITH TRIGGERED VLBI","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Gravitational microlensing; Physics; Astrophysics; Very Long Baseline Array; Very-long-baseline interferometry; Galaxy; Astronomy; Black hole (networking); Superluminal motion; Stars; Population; Active galactic nucleus","score_opus":0.006575309911233834,"score_gpt":0.19977587568238567,"score_spread":0.19320056577115183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2258780167","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9356079,0.00069006934,0.046863336,0.00028150086,0.000080961916,0.00016117776,0.0045322846,0.002689258,0.009093548],"genre_scores_gemma":[0.9712852,0.00007425074,0.024496818,0.00007874269,0.00005259856,0.00004636038,0.0032319608,0.00005814528,0.0006758431],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994842,0.00010345601,0.000019839792,0.0001443357,0.000121132405,0.00012687463],"domain_scores_gemma":[0.99922585,0.00014419125,0.00015411063,0.00016690609,0.000119887634,0.00018905634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000706514,0.0002496768,0.00036281534,0.0023104588,0.00025280204,0.0010862242,0.0005665416,0.00042980522,0.002485152],"category_scores_gemma":[0.0014187173,0.0002809209,0.0002301944,0.0013605166,0.00011927125,0.0005259304,0.000827344,0.0003725093,0.0006502545],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018697585,0.00069637306,0.49401826,0.00024446732,0.000850579,0.00058464316,0.00044998992,0.02131533,0.20682912,0.0066151083,0.010369676,0.25615668],"study_design_scores_gemma":[0.00019066225,0.00031795911,0.680535,0.000052436622,0.00020064508,0.0005205764,0.00026405076,0.25768235,0.03692739,0.006344771,0.016860979,0.000103076985],"about_ca_topic_score_codex":0.0039680596,"about_ca_topic_score_gemma":0.00693941,"teacher_disagreement_score":0.0039680596,"about_ca_system_score_codex":0.000634895,"about_ca_system_score_gemma":0.00031142178,"threshold_uncertainty_score":0.008313656},"labels":[],"label_agreement":null},{"id":"W2258807192","doi":"10.3847/1538-4357/835/2/140","title":"Ejection of the Massive Hydrogen-rich Envelope Timed with the Collapse of the Stripped SN 2014C","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":192,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"National Aeronautics and Space Administration","keywords":"Physics; Supernova; Astrophysics; Envelope (radar); Nucleosynthesis; Stellar evolution; Hydrogen; Ejecta; Astronomy; White dwarf; Binary number; Common envelope; Star (game theory); Stars","score_opus":0.008635430758977559,"score_gpt":0.21769949387911683,"score_spread":0.20906406312013928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2258807192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983865,0.00004772517,0.00014950821,0.000007633907,0.0000036455667,0.0000053910517,0.00051873876,0.000020593985,0.0008602107],"genre_scores_gemma":[0.99722517,0.000039221937,0.00028852635,0.000014607245,0.00000917428,0.0000064078145,0.0018904578,0.000007199417,0.00051927014],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988174,0.000006366756,0.0000069120633,0.00003134398,0.000046183486,0.000027480148],"domain_scores_gemma":[0.999511,0.000044982447,0.00014176354,0.000056234014,0.0001272418,0.00011873945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024352662,0.00020299024,0.0002471412,0.0013744726,0.00034279405,0.0005081449,0.00024023457,0.0001769949,0.000753616],"category_scores_gemma":[0.00060776045,0.00014252805,0.00022033624,0.0004878994,0.00022198331,0.00013549469,0.0005742868,0.00024144562,0.0002259933],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026453455,0.00007843301,0.9459621,0.000037790094,0.00012934921,0.00045736314,0.00018773232,0.0006511395,0.04132922,0.00032332414,0.00082591636,0.009753196],"study_design_scores_gemma":[0.000002096945,0.000029645325,0.9963043,0.000004003928,0.000013233665,0.00015661497,0.000043512933,0.00076624955,0.0018645106,0.000031717223,0.00077986834,0.000004328713],"about_ca_topic_score_codex":0.008726691,"about_ca_topic_score_gemma":0.015262798,"teacher_disagreement_score":0.008726691,"about_ca_system_score_codex":0.0004959558,"about_ca_system_score_gemma":0.00023769554,"threshold_uncertainty_score":0.017351806},"labels":[],"label_agreement":null},{"id":"W2261709274","doi":"10.3847/0004-637x/818/1/40","title":"TRIANGULUM II: A VERY METAL-POOR AND DYNAMICALLY HOT STELLAR SYSTEM","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Milky Way; Metallicity; Stars; Dwarf galaxy; Galaxy; Velocity dispersion; Radial velocity; Red-giant branch; Stellar kinematics; Astronomy; Satellite galaxy; Giant star","score_opus":0.007758617204485658,"score_gpt":0.2026902600016468,"score_spread":0.19493164279716116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2261709274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969778,0.000101471946,0.00023768861,0.000018182336,0.0000046396294,0.000007091092,0.00013519009,0.000012264829,0.0025057134],"genre_scores_gemma":[0.99810106,0.000039182556,0.00058312085,0.00001623789,0.0000069848156,0.0000037887228,0.000570886,0.0000070603737,0.0006716626],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983346,0.000012306869,0.000005022749,0.000054014276,0.000036874215,0.000058366495],"domain_scores_gemma":[0.99969256,0.00001626071,0.00006871545,0.00003585275,0.000027946075,0.00015853153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015864772,0.00022115582,0.00031232418,0.00084486976,0.001042248,0.0010067333,0.00056583306,0.00024099533,0.0015678677],"category_scores_gemma":[0.0003940163,0.00010116563,0.00012157284,0.000797659,0.0004046454,0.0003550429,0.0012834967,0.00026230433,0.0005000424],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003862591,0.00018713056,0.91709524,0.000055447093,0.00007195053,0.0019465571,0.001114845,0.0011681037,0.044069562,0.0041436316,0.001763809,0.02799749],"study_design_scores_gemma":[0.000032188,0.00050783844,0.9603289,0.00002292434,0.000033706398,0.0043074237,0.0017868457,0.0060894233,0.007143864,0.0010954258,0.018621866,0.000029633044],"about_ca_topic_score_codex":0.003043626,"about_ca_topic_score_gemma":0.0044956664,"teacher_disagreement_score":0.003043626,"about_ca_system_score_codex":0.0005898943,"about_ca_system_score_gemma":0.00023261586,"threshold_uncertainty_score":0.0060518384},"labels":[],"label_agreement":null},{"id":"W2262222539","doi":"10.3847/0004-637x/824/2/115","title":"AN ALL-SKY SEARCH FOR THREE FLAVORS OF NEUTRINOS FROM GAMMA-RAY BURSTS WITH THE ICECUBE NEUTRINO OBSERVATORY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":161,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; U.S. Department of Energy; Vetenskapsrådet; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; Western Canada Research Grid; Australian Research Council; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Vlaamse regering; University of Oxford; Compute Canada; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Neutrino; Cherenkov radiation; Muon; Gamma-ray burst; Observatory; Sky; Astrophysics; Neutrino astronomy; Cosmic ray; Neutrino detector; Astronomy; Astroparticle physics; COSMIC cancer database; Air shower; Solar neutrino; Particle physics; Neutrino oscillation; Detector","score_opus":0.019372200378922382,"score_gpt":0.2428176327410307,"score_spread":0.22344543236210831,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2262222539","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928029,0.0001321897,0.001492354,0.00005335367,0.000006599004,0.000028876066,0.0024320225,0.000058745933,0.0029928528],"genre_scores_gemma":[0.98720855,0.00012349099,0.0073651923,0.000051203635,0.000010617164,0.000035420766,0.0046840035,0.00002754739,0.0004940544],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969757,0.00007966544,0.000016678441,0.00007159588,0.000080556165,0.000053937445],"domain_scores_gemma":[0.9990282,0.00031000984,0.00022766662,0.00013264589,0.00013320455,0.00016832822],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010502331,0.00033693918,0.0002850754,0.001346783,0.0007296855,0.00078933174,0.0003289378,0.00023029253,0.0011036951],"category_scores_gemma":[0.0009169237,0.00018596227,0.00031085403,0.0011682983,0.00025171327,0.00033297262,0.0005717806,0.0002644352,0.00014284695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013318406,0.00019461369,0.8732265,0.00007137683,0.00031316545,0.0004438906,0.00036748865,0.003292109,0.088207036,0.0015213639,0.0015674791,0.029463094],"study_design_scores_gemma":[0.00021600565,0.0006184264,0.87822735,0.00005376462,0.00029828202,0.0009271121,0.00072373776,0.018759904,0.08394335,0.002145443,0.014025547,0.000061041064],"about_ca_topic_score_codex":0.0049558263,"about_ca_topic_score_gemma":0.009447015,"teacher_disagreement_score":0.0049558263,"about_ca_system_score_codex":0.00041326566,"about_ca_system_score_gemma":0.0005599991,"threshold_uncertainty_score":0.009853959},"labels":[],"label_agreement":null},{"id":"W2262857229","doi":"10.1088/0004-637x/806/2/229","title":"THE ENERGETICS OF CUSP DESTRUCTION","year":2015,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Halo; Dark matter halo; Dark matter; Cuspy halo problem; Scalar field dark matter; Galaxy; Light dark matter; Hot dark matter; Warm dark matter; Dark energy; Cosmology","score_opus":0.012423733131025468,"score_gpt":0.23887907045649304,"score_spread":0.22645533732546758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2262857229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9314433,0.0010724802,0.03301634,0.0002146752,0.00006827866,0.000017351593,0.00017162309,0.00015283337,0.03384305],"genre_scores_gemma":[0.9952034,0.00013743105,0.0023169739,0.000016332215,0.000009868357,0.0000071542645,0.00007704781,0.000046812416,0.00218507],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998215,0.000017487493,0.000009315338,0.00003298054,0.00006446786,0.00005429209],"domain_scores_gemma":[0.9993451,0.00024848335,0.00010024509,0.00012107167,0.00007918787,0.000105951236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004331527,0.00022537679,0.00027728023,0.00058469054,0.000600646,0.0010539567,0.00062852155,0.0003650556,0.004706346],"category_scores_gemma":[0.0021225156,0.00028090697,0.0004171744,0.00023175757,0.00054108637,0.000630075,0.001027017,0.0003620754,0.0007473778],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012251394,0.00012553786,0.16935301,0.00044430423,0.00017523748,0.0037722935,0.0011262165,0.24842957,0.21472968,0.21029979,0.002931038,0.14738823],"study_design_scores_gemma":[0.00008640332,0.00030989415,0.18610817,0.00009854817,0.00012662033,0.0046588033,0.000618249,0.6106585,0.0757564,0.10433391,0.017110018,0.00013446169],"about_ca_topic_score_codex":0.0007922597,"about_ca_topic_score_gemma":0.0006763683,"teacher_disagreement_score":0.004706346,"about_ca_system_score_codex":0.00087462267,"about_ca_system_score_gemma":0.00022711307,"threshold_uncertainty_score":0.015744328},"labels":[],"label_agreement":null},{"id":"W2264368166","doi":"10.1088/0004-637x/815/1/49","title":"BROADBAND RADIO POLARIMETRY AND FARADAY ROTATION OF 563 EXTRAGALACTIC RADIO SOURCES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Faraday effect; Physics; Faraday cage; Polarization (electrochemistry); Astrophysics; Polarimetry; Line-of-sight; Interstellar medium; Broadband; Galaxy; Telescope; Radio telescope; Optics; Astronomy; Scattering; Magnetic field","score_opus":0.013781376856533372,"score_gpt":0.22727755334469604,"score_spread":0.21349617648816266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2264368166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987644,0.00010892856,0.00016354749,0.000010557541,9.601458e-7,0.0000048327834,0.0004230724,0.000008148477,0.00051550916],"genre_scores_gemma":[0.9974178,0.0001378458,0.0003678397,0.00001060484,0.000007043701,0.0000069664343,0.0016315061,0.0000057159305,0.00041467635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998274,0.000022281794,0.000011934675,0.000046518766,0.000055628865,0.000036261965],"domain_scores_gemma":[0.9991441,0.00010400754,0.00037000686,0.00008893411,0.00013086112,0.00016200516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019197016,0.000277523,0.00029317098,0.002484625,0.00038752228,0.00057727186,0.00022157414,0.00022719537,0.0012117403],"category_scores_gemma":[0.0005758011,0.00024235295,0.00020292445,0.0018833346,0.00028175995,0.00028218093,0.0008035302,0.0002292152,0.0005656575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012495894,0.000032148622,0.96701515,0.000027697675,0.00006972458,0.00012110821,0.00069080415,0.00024920847,0.020379031,0.000087955894,0.00018919769,0.011012957],"study_design_scores_gemma":[0.00000208221,0.000007460977,0.99923563,0.0000018381888,0.000005958959,0.000058970465,0.000060209477,0.00006950527,0.00030129208,0.000012241387,0.00024295747,0.000001909967],"about_ca_topic_score_codex":0.0071201944,"about_ca_topic_score_gemma":0.011231722,"teacher_disagreement_score":0.0071201944,"about_ca_system_score_codex":0.00026053324,"about_ca_system_score_gemma":0.00011670558,"threshold_uncertainty_score":0.014157474},"labels":[],"label_agreement":null},{"id":"W2264947362","doi":"10.3847/0004-637x/827/1/59","title":"RADIO NONDETECTION OF THE SGR 1806−20 GIANT FLARE AND IMPLICATIONS FOR FAST RADIO BURSTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Astrophysics; Physics; Flare; Radio telescope; Fast radio burst; Astronomy; Fluence; Neutron star; Optics","score_opus":0.011341860604906584,"score_gpt":0.2956452152325392,"score_spread":0.2843033546276326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2264947362","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99788326,0.00013251851,0.00023639147,0.000084240404,0.000005897133,0.0000037004143,0.00034630203,0.000020649197,0.0012870259],"genre_scores_gemma":[0.9992855,0.000037955655,0.0001137484,0.00002525736,0.000013815575,0.000002102905,0.0004034535,0.000007969242,0.00011017831],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999652,0.000045705416,0.000038987768,0.00009936978,0.00009908211,0.000064880434],"domain_scores_gemma":[0.9954217,0.0012389768,0.002085954,0.00047347407,0.00041319677,0.00036666007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007332643,0.00023585747,0.00040775613,0.0015197253,0.0004621899,0.0012700428,0.0004944717,0.00040599253,0.0019544591],"category_scores_gemma":[0.0034830982,0.0001680354,0.00026747465,0.00084372144,0.0006916865,0.00055324566,0.0006564576,0.00036732876,0.00037147346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021310608,0.000029639787,0.9878791,0.000021544556,0.000028052138,0.00032752875,0.00012453517,0.0002884301,0.00654118,0.00024906904,0.00022729591,0.0040706214],"study_design_scores_gemma":[0.0000062173594,0.00003880447,0.99790573,0.000004753849,0.000010941201,0.00024728448,0.000070466864,0.00044394183,0.0007568922,0.00012354941,0.00038678368,0.0000047067256],"about_ca_topic_score_codex":0.0030944424,"about_ca_topic_score_gemma":0.003489997,"teacher_disagreement_score":0.0030944424,"about_ca_system_score_codex":0.00036509093,"about_ca_system_score_gemma":0.00011468508,"threshold_uncertainty_score":0.0065383315},"labels":[],"label_agreement":null},{"id":"W2265400054","doi":"10.3847/0004-637x/821/2/115","title":"SDSS-II SUPERNOVA SURVEY: AN ANALYSIS OF THE LARGEST SAMPLE OF TYPE IA SUPERNOVAE AND CORRELATIONS WITH HOST-GALAXY SPECTRAL PROPERTIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; U.S. Department of Energy; U.S. Naval Observatory; Los Alamos National Laboratory; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; York University; Universität Basel; Science and Technology Facilities Council; Fermilab; National Science Foundation; Case Western Reserve University; University of Pittsburgh; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Drexel University; National Aeronautics and Space Administration","keywords":"Supernova; Metallicity; Galaxy; Baryon; Hubble's law; Type (biology); Spectral line; Stellar mass; Stars","score_opus":0.018216759509968112,"score_gpt":0.2329506149300814,"score_spread":0.21473385542011328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2265400054","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99498934,0.00016814726,0.00025300457,0.00002337792,0.000005447566,0.000010607934,0.0042146724,0.00002150348,0.00031399462],"genre_scores_gemma":[0.9856167,0.00015670787,0.0005156923,0.000025043006,0.00001888331,0.000015253354,0.013447867,0.00002099011,0.00018295446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989937,0.00022470366,0.0001717718,0.00026904332,0.00022907525,0.00011170626],"domain_scores_gemma":[0.99426705,0.0011867535,0.0018995634,0.0008367877,0.00071544386,0.001094388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021031718,0.00047351883,0.0007261037,0.0045938855,0.00038497336,0.00096839375,0.00046110674,0.00029736533,0.001515419],"category_scores_gemma":[0.003192747,0.00027265612,0.0007789718,0.003981952,0.00029453504,0.00039134838,0.0011806446,0.00036575107,0.00058739516],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000341794,0.000019347492,0.998054,0.000010691957,0.00012405425,0.00002861728,0.000022702972,0.000073476156,0.0005461571,0.000025620924,0.00023635301,0.0008247285],"study_design_scores_gemma":[0.0000036705217,0.000018509061,0.9992223,0.0000031323682,0.000031401643,0.00008246904,0.000051446335,0.00018147526,0.0001450952,0.000007713459,0.00025034725,0.000002327985],"about_ca_topic_score_codex":0.007275764,"about_ca_topic_score_gemma":0.0116768265,"teacher_disagreement_score":0.007275764,"about_ca_system_score_codex":0.00024691838,"about_ca_system_score_gemma":0.0004595752,"threshold_uncertainty_score":0.014466822},"labels":[],"label_agreement":null},{"id":"W2266617027","doi":"10.3847/1538-4357/836/1/13","title":"Properties and Alignment of Interstellar Dust Grains toward Type Ia Supernovae with Anomalous Polarization Curves","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Supernova; Polarization (electrochemistry); Cosmic dust; Interstellar medium; Radiative transfer; Extinction (optical mineralogy); Polarimetry; Wavelength; Galaxy","score_opus":0.023434599632081995,"score_gpt":0.2347335658072763,"score_spread":0.2112989661751943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2266617027","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992298,0.000010560598,0.00051375217,0.0000014345443,3.4586927e-7,8.855799e-7,0.000062202584,0.000010815779,0.00017017433],"genre_scores_gemma":[0.9996265,0.0000048002107,0.00019410574,9.518645e-7,5.015782e-7,8.3390177e-7,0.00014276932,0.000002120882,0.000027383046],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989784,0.000014105866,0.000010134846,0.000038182723,0.000020343505,0.000019302695],"domain_scores_gemma":[0.9994049,0.00015403362,0.00022289708,0.00006332786,0.00009594522,0.00005892272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021585866,0.00025375857,0.00013956419,0.0009831416,0.00015456295,0.00042280622,0.00020710262,0.00024083062,0.00052271737],"category_scores_gemma":[0.0007435215,0.00016971164,0.00026441904,0.00043407464,0.00021525173,0.00017772548,0.0001906953,0.000109916604,0.00013784062],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000082510596,0.0000133388785,0.95735437,0.000006697698,0.00004383296,0.00007319912,0.00003596267,0.003024496,0.037252996,0.00009505202,0.00003198223,0.0019856466],"study_design_scores_gemma":[0.0000024526971,0.000030382393,0.9782869,0.0000016030723,0.000018482573,0.00019668002,0.00006716533,0.013065704,0.008153599,0.000090290116,0.00008262785,0.0000040202117],"about_ca_topic_score_codex":0.0017712867,"about_ca_topic_score_gemma":0.0014030394,"teacher_disagreement_score":0.0017712867,"about_ca_system_score_codex":0.00019909484,"about_ca_system_score_gemma":0.000066254834,"threshold_uncertainty_score":0.0035219193},"labels":[],"label_agreement":null},{"id":"W2266746071","doi":"10.1088/0004-637x/725/1/496","title":"EXPLORING SHORT GAMMA-RAY BURSTS AS GRAVITATIONAL-WAVE STANDARD SIRENS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":426,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Gravitational wave; Neutron star; Astrophysics; Cosmic distance ladder; Luminosity distance; Redshift; Binary number; Sky; Coalescence (physics); LIGO; Astronomy; Galaxy","score_opus":0.03758089546606445,"score_gpt":0.25789649808384035,"score_spread":0.2203156026177759,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2266746071","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9140782,0.00027041015,0.082816236,0.00018203245,0.0000054492343,0.00002443475,0.00014324415,0.00007136765,0.002408687],"genre_scores_gemma":[0.9894628,0.00023209161,0.00960675,0.000023506684,0.000010031956,0.000019690944,0.0001375042,0.000019028887,0.0004886484],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996176,0.00018640862,0.000014657238,0.000087352135,0.00006193709,0.00003198002],"domain_scores_gemma":[0.9919844,0.005942913,0.0011386955,0.00049854437,0.00020151316,0.00023393064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002528136,0.0002452937,0.0002869739,0.00097256433,0.00031196943,0.0018498033,0.0006610482,0.00050821074,0.0011079579],"category_scores_gemma":[0.011569366,0.000438399,0.00028189507,0.0008167579,0.001221485,0.0024543689,0.0011882603,0.00060498004,0.00012810038],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003946783,0.00013469314,0.28474566,0.00008600046,0.00015433546,0.0003587543,0.0013029999,0.22893043,0.007977058,0.42186618,0.00072502607,0.053324297],"study_design_scores_gemma":[0.000033586337,0.00007337764,0.06065514,0.00003671684,0.000036369,0.0002414861,0.0002324332,0.7379873,0.0020509714,0.19673453,0.0018700158,0.0000480418],"about_ca_topic_score_codex":0.0020203248,"about_ca_topic_score_gemma":0.0021013212,"teacher_disagreement_score":0.002528136,"about_ca_system_score_codex":0.0008042878,"about_ca_system_score_gemma":0.00031838723,"threshold_uncertainty_score":0.013370216},"labels":[],"label_agreement":null},{"id":"W2267382154","doi":"10.3847/0004-637x/830/1/36","title":"AN ECCENTRIC BINARY MILLISECOND PULSAR WITH A HELIUM WHITE DWARF COMPANION IN THE GALACTIC FIELD","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Millisecond pulsar; Astrophysics; White dwarf; Pulsar; Neutron star; Accretion (finance); Eccentricity (behavior); Astronomy; Orbital eccentricity; Stars","score_opus":0.008577224080625502,"score_gpt":0.22709357828588883,"score_spread":0.21851635420526333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2267382154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995228,0.00003738207,0.000046468023,0.000023872719,0.0000034671868,0.0000018403626,0.000012904283,0.0000021594403,0.00034908153],"genre_scores_gemma":[0.9998276,0.00000968949,0.000017283008,0.0000089771975,0.0000056071885,3.9270253e-7,0.000015183511,3.605497e-7,0.00011488742],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999378,0.000008160938,0.0000059217537,0.000017112821,0.000010272996,0.000020701738],"domain_scores_gemma":[0.99982053,0.00002814196,0.00005426057,0.000014366079,0.000013408497,0.000069464615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014780393,0.00023404251,0.00024111393,0.0007692373,0.0007902499,0.0004088491,0.0001880924,0.00038059847,0.00098009],"category_scores_gemma":[0.00040182908,0.00011674877,0.00011578191,0.00042662473,0.0003266895,0.0002090391,0.00037638663,0.00019116081,0.00017459328],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005039391,0.00023534877,0.93371254,0.000017815657,0.000055323897,0.049427148,0.00048641197,0.00034133784,0.0088521615,0.00031624307,0.00023572973,0.0058158985],"study_design_scores_gemma":[0.000055064782,0.0005070395,0.94987494,0.000007717976,0.00004734805,0.042805463,0.0010987904,0.001581608,0.002549597,0.0003790404,0.0010808994,0.000012335549],"about_ca_topic_score_codex":0.0036149484,"about_ca_topic_score_gemma":0.003319128,"teacher_disagreement_score":0.0036149484,"about_ca_system_score_codex":0.0002789757,"about_ca_system_score_gemma":0.00012830258,"threshold_uncertainty_score":0.0071878433},"labels":[],"label_agreement":null},{"id":"W2267820293","doi":"10.1088/0004-637x/725/2/2087","title":"ANISOTROPIC GALACTIC OUTFLOWS AND ENRICHMENT OF THE INTERGALACTIC MEDIUM. II. NUMERICAL SIMULATIONS","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Anisotropy; Physics; Astrophysics; Intergalactic travel; Intergalactic medium; Intergalactic dust; Galaxy; Optics; Redshift","score_opus":0.005771181537685191,"score_gpt":0.22067644943073417,"score_spread":0.21490526789304898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2267820293","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94533163,0.00042045733,0.03566114,0.00051028695,0.00006978857,0.00013139204,0.0014299224,0.00036895912,0.016076429],"genre_scores_gemma":[0.98430586,0.00023848463,0.0123838885,0.00014885893,0.000027652579,0.00011854528,0.0006179936,0.00007492631,0.0020837185],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997632,0.00006963122,0.000011816243,0.000037148267,0.000044437682,0.00007379182],"domain_scores_gemma":[0.99929774,0.00026001062,0.00014937532,0.000078879086,0.00010262158,0.0001114594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048919267,0.0006010666,0.0007925943,0.000687531,0.00060045085,0.001389941,0.0015515492,0.0016982865,0.0024433983],"category_scores_gemma":[0.0026528551,0.000495446,0.00082510576,0.0008329394,0.00086181704,0.00098353,0.0008833156,0.00089704274,0.0002845334],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004455512,0.00003915212,0.0062418007,0.000017462451,0.000019476965,0.0000663124,0.00003112995,0.98785794,0.0007974722,0.003893471,0.00017838713,0.00081291446],"study_design_scores_gemma":[0.000039367977,0.000015155259,0.0010484265,0.000007246263,0.0000078532275,0.000020260259,0.00002584542,0.99640095,0.0003254509,0.0016358847,0.00046519918,0.000008310512],"about_ca_topic_score_codex":0.02495134,"about_ca_topic_score_gemma":0.007947158,"teacher_disagreement_score":0.02495134,"about_ca_system_score_codex":0.0016834242,"about_ca_system_score_gemma":0.0009127181,"threshold_uncertainty_score":0.049612224},"labels":[],"label_agreement":null},{"id":"W2268561420","doi":"10.1088/0004-637x/815/2/120","title":"METAMORPHOSIS OF SN 2014C: DELAYED INTERACTION BETWEEN A HYDROGEN POOR CORE-COLLAPSE SUPERNOVA AND A NEARBY CIRCUMSTELLAR SHELL","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Supernova; Red supergiant; Astronomy; Stars; Supergiant","score_opus":0.02885286287108624,"score_gpt":0.2560647533460241,"score_spread":0.22721189047493784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2268561420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99846965,0.000046880446,0.00010131538,0.000010115613,0.0000065609647,0.000015319094,0.00024518874,0.000016727716,0.0010883204],"genre_scores_gemma":[0.99834895,0.00003152569,0.0002980587,0.000015713711,0.000008271705,0.000007303765,0.00089194294,0.0000054212464,0.00039269734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998795,0.000005556869,0.000008101543,0.00003582442,0.00003701537,0.000033991582],"domain_scores_gemma":[0.9996555,0.000016924841,0.000104248706,0.00002962317,0.00004608791,0.00014757669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017388602,0.00034914672,0.00034158022,0.0010727855,0.00065994,0.0005511375,0.0002851855,0.000321329,0.00074274244],"category_scores_gemma":[0.00038403957,0.0002148939,0.00025552727,0.0004587701,0.0002733469,0.00021059834,0.00071342883,0.00038598044,0.0001453698],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044716097,0.00015647369,0.91371167,0.000038131067,0.00011425697,0.0025632796,0.000166984,0.0005215019,0.07210468,0.00047777995,0.0006727831,0.009025301],"study_design_scores_gemma":[0.000006171208,0.00011908305,0.9931543,0.000005127903,0.000012483885,0.001960454,0.00006674019,0.00076981145,0.0030067824,0.000063363346,0.00082902703,0.00000666126],"about_ca_topic_score_codex":0.011401134,"about_ca_topic_score_gemma":0.02869576,"teacher_disagreement_score":0.011401134,"about_ca_system_score_codex":0.00078569737,"about_ca_system_score_gemma":0.0003692093,"threshold_uncertainty_score":0.022669554},"labels":[],"label_agreement":null},{"id":"W2268739927","doi":"10.3847/0004-637x/820/1/69","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. VII. THE INTRINSIC SHAPES OF LOW-LUMINOSITY GALAXIES IN THE CORE OF THE VIRGO CLUSTER, AND A COMPARISON WITH THE LOCAL GROUP","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Herzberg Institute of Astrophysics","funders":"","keywords":"Virgo Cluster; Galaxy; Cluster (spacecraft); Population; Galaxy cluster; Local Group; Core (optical fiber)","score_opus":0.019748314305279485,"score_gpt":0.22236650631286034,"score_spread":0.20261819200758086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2268739927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99656564,0.00014207994,0.00021175883,0.000029672905,0.0000013009455,0.0000065179297,0.0022751873,0.000020107833,0.0007476936],"genre_scores_gemma":[0.9929543,0.000061432824,0.0007952277,0.000020087178,0.0000033947063,0.000007592488,0.005811071,0.000010477123,0.00033640413],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998561,0.000029129062,0.000005651322,0.000042113432,0.000035579804,0.000031330506],"domain_scores_gemma":[0.99961746,0.000044415527,0.00010968015,0.00007381295,0.00005052025,0.00010415371],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041373,0.0001743095,0.00016358415,0.0012447888,0.00020917488,0.00038223033,0.00023794928,0.00020084382,0.0005698413],"category_scores_gemma":[0.00059573544,0.0001227545,0.00022061625,0.0007369874,0.0001973289,0.00024801504,0.0005344106,0.00014876414,0.00033617727],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000080213504,0.000022644577,0.9881753,0.000014582229,0.00003955281,0.000035457957,0.0001528211,0.000717643,0.0027717862,0.0002037979,0.000810896,0.0069754035],"study_design_scores_gemma":[0.0000017544726,0.000007416711,0.9983919,0.0000022811016,0.0000051355637,0.000037761667,0.000041619238,0.00077389675,0.00019725802,0.000042975444,0.00049575244,0.0000022432237],"about_ca_topic_score_codex":0.01658764,"about_ca_topic_score_gemma":0.036765557,"teacher_disagreement_score":0.01658764,"about_ca_system_score_codex":0.0004874778,"about_ca_system_score_gemma":0.00015267267,"threshold_uncertainty_score":0.03298217},"labels":[],"label_agreement":null},{"id":"W2269309009","doi":"10.3847/0004-637x/820/1/32","title":"THE FIRST BROWN DWARF/PLANETARY-MASS OBJECT IN THE 32 ORIONIS GROUP*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Sky; Stars; Proper motion; Stellar classification; Radial velocity; Infrared; Object (grammar)","score_opus":0.00828254911797197,"score_gpt":0.21336971980470495,"score_spread":0.205087170686733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2269309009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99798405,0.000052666193,0.00018638038,0.000027402712,0.0000075550884,0.0000034008729,0.000053801825,0.000020222938,0.001664372],"genre_scores_gemma":[0.998497,0.000018175204,0.0005056836,0.000024233872,0.000011886013,0.0000023840953,0.00021071195,0.000005645794,0.00072415214],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992394,0.00000550686,0.000004626551,0.000025015814,0.000019481664,0.000021421822],"domain_scores_gemma":[0.99979275,0.000016355318,0.000058557744,0.000027644977,0.00001801049,0.0000866906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014847759,0.00020744906,0.00016951821,0.0004688706,0.00056705566,0.00037686166,0.00025498017,0.00026533703,0.001757582],"category_scores_gemma":[0.0002907005,0.00009871885,0.000097240874,0.00027892995,0.00025075415,0.00022723914,0.00067947985,0.00026461022,0.0005148525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026595528,0.00012065858,0.849017,0.00005753288,0.00003725522,0.004512407,0.0011701151,0.0001240948,0.109924376,0.0011126768,0.0014258925,0.03223213],"study_design_scores_gemma":[0.000013024246,0.00022714397,0.9643894,0.000013945646,0.000022711654,0.0052691866,0.00042882265,0.00048230035,0.01184128,0.0004722219,0.016831001,0.000008978501],"about_ca_topic_score_codex":0.0007415571,"about_ca_topic_score_gemma":0.0010045461,"teacher_disagreement_score":0.001757582,"about_ca_system_score_codex":0.00017612369,"about_ca_system_score_gemma":0.00012257847,"threshold_uncertainty_score":0.00587976},"labels":[],"label_agreement":null},{"id":"W2269355149","doi":"10.1088/0004-637x/805/1/51","title":"A MEGACAM SURVEY OF OUTER HALO SATELLITES. IV. TWO FOREGROUND POPULATIONS POSSIBLY ASSOCIATED WITH THE MONOCEROS SUBSTRUCTURE IN THE DIRECTION OF NGC 2419 AND KOPOSOV 2","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Comisión Nacional de Investigación Científica y Tecnológica; National Science Foundation","keywords":"Globular cluster; Galactic halo; Milky Way; Halo; Metallicity; Population; Stellar population","score_opus":0.034137359300420146,"score_gpt":0.25902032821940024,"score_spread":0.2248829689189801,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2269355149","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99718434,0.00009739181,0.00009593238,0.0000132502055,0.0000016761246,0.000004997469,0.00083261816,0.000007415657,0.0017624383],"genre_scores_gemma":[0.99641466,0.000061257306,0.0005636992,0.000010373177,0.0000033712668,0.000004611571,0.0020263875,0.0000031635013,0.0009126181],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999225,0.000009091446,0.000003098334,0.000019809899,0.000023880877,0.000021580996],"domain_scores_gemma":[0.99975616,0.000013623294,0.00006457902,0.000026706866,0.000049379534,0.00008952273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017330701,0.00008547054,0.00009904321,0.0008408501,0.00026949277,0.00021531146,0.0001690522,0.00009043954,0.0011992222],"category_scores_gemma":[0.0002338206,0.00008087188,0.00010740507,0.00058569206,0.000090379624,0.00012021474,0.00042232627,0.00007728129,0.0002177451],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010307102,0.000014428716,0.97643423,0.000022552136,0.00003448031,0.00015292662,0.00027049985,0.00013746454,0.009141415,0.0003538743,0.00068246864,0.012652595],"study_design_scores_gemma":[0.0000025171723,0.000007390271,0.998336,0.0000031139184,0.000004235753,0.0000446877,0.000078315454,0.00016512208,0.00030551403,0.000019288726,0.0010330494,7.4969466e-7],"about_ca_topic_score_codex":0.021494579,"about_ca_topic_score_gemma":0.07432998,"teacher_disagreement_score":0.021494579,"about_ca_system_score_codex":0.0003872588,"about_ca_system_score_gemma":0.00022962884,"threshold_uncertainty_score":0.042738914},"labels":[],"label_agreement":null},{"id":"W2269789618","doi":"10.3847/0004-637x/821/1/18","title":"ON THE MASS AND ORIGIN OF CHARIKLO’S RINGS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Centaur; Physics; Eccentricity (behavior); Ring (chemistry); Astrophysics; Longitude; Planet; Precession; Solar System; Orbit (dynamics); Astronomy; Latitude; Chemistry","score_opus":0.009833520610324753,"score_gpt":0.20626943630173172,"score_spread":0.19643591569140698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2269789618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984837,0.00014411754,0.000092008304,0.000022293674,0.0000031924696,0.0000015470081,0.000060192113,0.000007222196,0.0011856148],"genre_scores_gemma":[0.99984133,0.000015298545,0.00003540621,0.0000021094434,0.000002079978,4.407601e-7,0.000031228028,0.0000011346,0.000071094284],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99986386,0.00001863389,0.0000059942345,0.00003498506,0.000019798896,0.000056699504],"domain_scores_gemma":[0.9986523,0.00022652707,0.00058153307,0.00008753635,0.0001912327,0.0002609928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004837665,0.00011239196,0.00010810903,0.001663442,0.0006194911,0.00120596,0.00041437932,0.00017506888,0.0012421404],"category_scores_gemma":[0.0012301052,0.0001279451,0.0001248425,0.00045746262,0.0005504975,0.00030692795,0.00061910803,0.00017331743,0.00026300954],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032920486,0.000020830379,0.976219,0.00002655715,0.000024752311,0.0005391894,0.0007329703,0.00041904545,0.01332338,0.0012896054,0.00022378714,0.006851652],"study_design_scores_gemma":[0.0000038065039,0.00003572442,0.99582833,0.000011912223,0.0000096391705,0.00030048128,0.00040420468,0.00075278775,0.0016456336,0.00015884146,0.0008399056,0.00000874309],"about_ca_topic_score_codex":0.0043446627,"about_ca_topic_score_gemma":0.005031986,"teacher_disagreement_score":0.0043446627,"about_ca_system_score_codex":0.0008708233,"about_ca_system_score_gemma":0.00022242549,"threshold_uncertainty_score":0.00863874},"labels":[],"label_agreement":null},{"id":"W2269943929","doi":"10.3847/0004-637x/821/2/98","title":"THE JCMT GOULD BELT SURVEY: DENSE CORE CLUSTERS IN ORION B","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Waterloo; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"James Clerk Maxwell Telescope; Core (optical fiber); Telescope; Cluster (spacecraft); Cluster analysis; Correlation function (quantum field theory)","score_opus":0.02116972497379914,"score_gpt":0.2596772885169645,"score_spread":0.23850756354316532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2269943929","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99834895,0.00010306902,0.000039576218,0.0000462486,0.0000012560118,0.0000067682267,0.00082866795,0.000012160579,0.0006132299],"genre_scores_gemma":[0.9976427,0.00007872112,0.00028107225,0.000033310534,0.000006868742,0.0000068824597,0.0015877169,0.000007175843,0.00035546723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999782,0.0000243064,0.0000135915925,0.000054819167,0.00007456949,0.000050673145],"domain_scores_gemma":[0.9990651,0.00008938358,0.0003222601,0.00010364969,0.00008470314,0.00033489242],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003860925,0.0001240076,0.00018172419,0.0028375553,0.0005385127,0.00039371575,0.00034851435,0.00019432929,0.0009848638],"category_scores_gemma":[0.0010288174,0.00011028364,0.00010818906,0.0019786526,0.00032920667,0.00027370392,0.0010265714,0.00013704614,0.00020988789],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079945334,0.000027571066,0.98858297,0.00001802867,0.000027727801,0.000107380896,0.0006969672,0.00008080953,0.0034024809,0.00016104891,0.0010635627,0.0057515455],"study_design_scores_gemma":[0.0000023611308,0.0000030526091,0.99929035,0.0000027174763,0.0000023584394,0.000019975188,0.000086906155,0.000041913994,0.000065119435,0.00001486253,0.0004693362,9.460123e-7],"about_ca_topic_score_codex":0.075293384,"about_ca_topic_score_gemma":0.14327198,"teacher_disagreement_score":0.075293384,"about_ca_system_score_codex":0.0006737785,"about_ca_system_score_gemma":0.00036479553,"threshold_uncertainty_score":0.1497103},"labels":[],"label_agreement":null},{"id":"W2272085088","doi":"10.3847/0004-637x/821/2/78","title":"THE OPTICAL–INFRARED EXTINCTION CURVE AND ITS VARIATION IN THE MILKY WAY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":243,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Chinese Academy of Sciences; Deutsche Forschungsgemeinschaft; Queen's University Belfast; Space Telescope Science Institute; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Universität Basel; Fermilab; National Science Foundation; Case Western Reserve University; University of Pittsburgh; Los Alamos National Laboratory; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Queen's University; Ohio State University; Durham University; Drexel University; U.S. Naval Observatory; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Milky Way; Extinction (optical mineralogy); Photometry (optics); Light curve; Molecular cloud; Infrared; Interstellar medium","score_opus":0.010552052264071892,"score_gpt":0.23087953464225772,"score_spread":0.22032748237818583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2272085088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99702054,0.00007528216,0.00043535102,0.00002492905,0.0000017368321,0.0000018576108,0.00057250157,0.000058877748,0.0018087907],"genre_scores_gemma":[0.99882096,0.000024604848,0.00025023622,0.000012439485,0.0000035036353,0.0000020961982,0.0006070094,0.000013658895,0.00026549908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998721,0.00001894233,0.0000073438605,0.000046599485,0.000034842542,0.000020136527],"domain_scores_gemma":[0.9992772,0.00015803239,0.00026880417,0.00008950151,0.0001203945,0.00008596104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025777603,0.00012404745,0.00013284368,0.0011288776,0.00011222938,0.00041577846,0.00015799435,0.00014945726,0.0009262586],"category_scores_gemma":[0.00091989676,0.00008406984,0.00017389083,0.00079396286,0.00021785994,0.00040279442,0.00030566962,0.0001694421,0.00028661705],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046039182,0.000028513436,0.98475236,0.000011026046,0.000064478045,0.00006213923,0.000119651726,0.001321822,0.0046617007,0.0002306563,0.00061587937,0.008085801],"study_design_scores_gemma":[0.0000011907642,0.0000065505774,0.9982065,0.0000016067706,0.000004547143,0.000033768316,0.000034133704,0.0007903638,0.0003348012,0.000070405404,0.0005140857,0.0000020444606],"about_ca_topic_score_codex":0.0041587236,"about_ca_topic_score_gemma":0.0034743208,"teacher_disagreement_score":0.0041587236,"about_ca_system_score_codex":0.00022873729,"about_ca_system_score_gemma":0.00007207356,"threshold_uncertainty_score":0.008269072},"labels":[],"label_agreement":null},{"id":"W2272392192","doi":"10.3847/1538-4357/834/2/126","title":"DHIGLS: DRAO H i INTERMEDIATE GALACTIC LATITUDE SURVEY","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Herzberg Institute of Astrophysics; Université Laval; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Spectral line; Galactic plane; Angular resolution (graph drawing); Galactic Center; Green Bank Telescope; Interstellar medium; Telescope; Radio telescope; Latitude","score_opus":0.022889122878379152,"score_gpt":0.28283403332465185,"score_spread":0.2599449104462727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2272392192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.49049464,0.000535249,0.0017889068,0.00047091403,0.00009005647,0.00025356986,0.46240583,0.0042866073,0.03967427],"genre_scores_gemma":[0.48023266,0.00023221568,0.0070871953,0.0005327596,0.00007768269,0.00021459743,0.5021589,0.0004538182,0.009010216],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999814,0.000018650953,0.000008887623,0.00005157572,0.00006856315,0.00003835817],"domain_scores_gemma":[0.9995121,0.000020634987,0.00011361501,0.00008775654,0.00010726787,0.00015858698],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003136048,0.00034889902,0.00021617107,0.0017953867,0.00021815322,0.0004975952,0.0006636739,0.00019003858,0.005386013],"category_scores_gemma":[0.0004264267,0.000120603974,0.00020694373,0.0013255823,0.00014425229,0.00020967668,0.0006806993,0.00025141655,0.0025087462],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009698202,0.00020264195,0.67927337,0.00042886822,0.0003566854,0.00067423814,0.0006241175,0.002840975,0.031268243,0.0015995901,0.20758964,0.074171826],"study_design_scores_gemma":[0.00013819114,0.00008195484,0.86806774,0.00003978603,0.00004101814,0.00012527204,0.00026155912,0.001136233,0.0029163172,0.00025364163,0.1269164,0.000021842778],"about_ca_topic_score_codex":0.035063468,"about_ca_topic_score_gemma":0.052537646,"teacher_disagreement_score":0.035063468,"about_ca_system_score_codex":0.0007728173,"about_ca_system_score_gemma":0.0005039866,"threshold_uncertainty_score":0.06971878},"labels":[],"label_agreement":null},{"id":"W2272649649","doi":"10.3847/0004-637x/817/1/23","title":"ETA CARINAE’S THERMAL X-RAY TAIL MEASURED WITH XMM-NEWTON AND NuSTAR","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Goddard Space Flight Center; Science and Technology Facilities Council; Oak Ridge Associated Universities; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; X-ray; X-ray background; Thermal; Astronomy; X-ray astronomy; Active galactic nucleus; Nuclear physics; Galaxy","score_opus":0.011498283397999083,"score_gpt":0.2023125438279507,"score_spread":0.19081426042995162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2272649649","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99851733,0.00006227168,0.00007269647,0.000007881272,0.0000015369426,0.0000018453059,0.00019737182,0.000014801179,0.0011242706],"genre_scores_gemma":[0.99906486,0.000026504811,0.0001346331,0.0000079304355,0.0000028470286,0.0000020181524,0.00036520435,0.000003263854,0.00039274458],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999324,0.000004848634,0.00000407053,0.000027595206,0.000017071361,0.000014104122],"domain_scores_gemma":[0.99970347,0.000025995287,0.00009312307,0.000031284584,0.00007130337,0.00007485732],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016342122,0.0001544853,0.00015997492,0.0008193572,0.00037201316,0.00047288262,0.00017901977,0.00022016172,0.001128832],"category_scores_gemma":[0.00037722776,0.00014237808,0.00011803327,0.00035413407,0.00016619464,0.00022358047,0.0003823424,0.00016126662,0.0004008936],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012185075,0.000023312714,0.9680332,0.000016227239,0.00002852574,0.0003050186,0.00031409287,0.00017580511,0.026839036,0.0000842309,0.000173686,0.00388493],"study_design_scores_gemma":[6.2103334e-7,0.000016787286,0.99838257,0.0000016729502,0.0000030184092,0.00016880294,0.00007785812,0.00019175898,0.0008035658,0.0000122223555,0.00033961918,0.0000014983134],"about_ca_topic_score_codex":0.002663365,"about_ca_topic_score_gemma":0.006184104,"teacher_disagreement_score":0.002663365,"about_ca_system_score_codex":0.00025016864,"about_ca_system_score_gemma":0.00008219076,"threshold_uncertainty_score":0.0052957535},"labels":[],"label_agreement":null},{"id":"W2274577657","doi":"10.1088/0004-637x/810/1/78","title":"A COUPLED 2 × 2D BABCOCK–LEIGHTON SOLAR DYNAMO MODEL. I. SURFACE MAGNETIC FLUX EVOLUTION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Collège de Bois-de-Boulogne","funders":"","keywords":"Dynamo; Magnetogram; Solar dynamo; Dipole; Meridional flow; Series (stratigraphy); Magnetic flux; Solar cycle","score_opus":0.009847489161666534,"score_gpt":0.21869676270075972,"score_spread":0.2088492735390932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2274577657","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7681035,0.001238668,0.14224957,0.003611059,0.0003984881,0.0001716819,0.002840969,0.0005710572,0.080815084],"genre_scores_gemma":[0.97877717,0.00029181782,0.007040682,0.00023616177,0.00007856756,0.00018229338,0.0005208691,0.00007248046,0.012799908],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999887,0.00003460839,0.0000059341046,0.000038837927,0.000015424033,0.000018234628],"domain_scores_gemma":[0.99971646,0.00010411557,0.00004562035,0.00002238041,0.000044109693,0.00006733357],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026152396,0.0005261778,0.0009228003,0.00038568655,0.00063830777,0.001362653,0.0014881961,0.001951122,0.004341883],"category_scores_gemma":[0.0009595325,0.0005296072,0.0008057753,0.0004994341,0.0009698467,0.00091807544,0.0010896225,0.0009354429,0.00046231438],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006680117,0.000025473188,0.0015626216,0.000021956454,0.00003608495,0.00012036315,0.000044236793,0.984268,0.0009089825,0.011118059,0.00063259527,0.0011948225],"study_design_scores_gemma":[0.00002471151,0.000009611056,0.0003673779,0.0000021363617,0.000007960842,0.000013819399,0.000010716101,0.99660945,0.000039711886,0.0025664682,0.00034056968,0.0000074671448],"about_ca_topic_score_codex":0.029843705,"about_ca_topic_score_gemma":0.009659687,"teacher_disagreement_score":0.029843705,"about_ca_system_score_codex":0.001303019,"about_ca_system_score_gemma":0.0008618441,"threshold_uncertainty_score":0.05934},"labels":[],"label_agreement":null},{"id":"W2274945749","doi":"10.3847/0004-637x/832/1/13","title":"TYPE Ia SUPERNOVA EXPLOSIONS FROM HYBRID CARBON–OXYGEN–NEON WHITE DWARF PROGENITORS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supernova; White dwarf; Stars; Thermonuclear fusion; Stellar evolution; Code (set theory)","score_opus":0.013281999879913913,"score_gpt":0.23162040116854077,"score_spread":0.21833840128862686,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2274945749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968111,0.000027063781,0.0015496158,0.000019309875,0.00000768842,0.000012888225,0.00012682925,0.00006240418,0.0013830839],"genre_scores_gemma":[0.99789447,0.00003549828,0.0013759829,0.000017936787,0.000004148565,0.000017014616,0.0003139009,0.000021808646,0.00031912248],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988425,0.000025390505,0.000008657514,0.000021418398,0.000025899364,0.000034389937],"domain_scores_gemma":[0.9993549,0.00032382924,0.00009269407,0.000059639548,0.00007451717,0.00009448778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042619221,0.0004672298,0.00043690504,0.00043020878,0.0004181325,0.00056641066,0.0006638814,0.00041803502,0.000846281],"category_scores_gemma":[0.0014712772,0.00019696273,0.0006532821,0.00039715838,0.0004478923,0.00031750937,0.00062186056,0.0005126907,0.000086186934],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019374196,0.00011581787,0.029215897,0.000028869075,0.00010544643,0.00032911325,0.00007112877,0.9624395,0.0028216222,0.0021947245,0.00032201066,0.0021621198],"study_design_scores_gemma":[0.000109261855,0.0001539272,0.008586243,0.000008671589,0.000029123144,0.00007861128,0.00008555581,0.98623127,0.0032794194,0.0009747742,0.00044903392,0.000014115842],"about_ca_topic_score_codex":0.00947545,"about_ca_topic_score_gemma":0.008557574,"teacher_disagreement_score":0.00947545,"about_ca_system_score_codex":0.0006710735,"about_ca_system_score_gemma":0.00041923506,"threshold_uncertainty_score":0.018840551},"labels":[],"label_agreement":null},{"id":"W2275004005","doi":"10.3847/1538-4357/835/2/160","title":"Cosmic Voids in the SDSS DR12 BOSS Galaxy Sample: the Alcock–Paczyński test","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Boss; Redshift; Galaxy; Void (composites); Baryon; COSMIC cancer database; Measure (data warehouse); Line-of-sight; Photometric redshift","score_opus":0.012153113929773075,"score_gpt":0.24239244770894572,"score_spread":0.23023933377917263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2275004005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99657273,0.00006341757,0.0018492044,0.00006111122,0.000006782809,0.000008683407,0.00051875325,0.000054014516,0.000865344],"genre_scores_gemma":[0.9989058,0.000008513245,0.00037893452,0.000016143904,0.000008614944,0.0000080123555,0.0005998351,0.000012195637,0.00006194826],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9964097,0.0009726332,0.0003324309,0.0008900742,0.0009641419,0.00043096213],"domain_scores_gemma":[0.9705813,0.013700551,0.0073230616,0.0044282605,0.0014433364,0.0025235089],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004261811,0.00032424228,0.0005143645,0.002418124,0.0006077847,0.0016446303,0.0011376662,0.0006564095,0.0026854505],"category_scores_gemma":[0.028826388,0.00020245195,0.00052853907,0.0018577077,0.0017678408,0.0015667657,0.0020086304,0.00063032424,0.00045642836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032311966,0.000040600335,0.9873324,0.000021832084,0.00019180626,0.00010235795,0.0001943265,0.00207775,0.0013325267,0.0015769077,0.00084771425,0.005958735],"study_design_scores_gemma":[0.000033503107,0.00009272506,0.9764297,0.000013258617,0.000054148444,0.00022872828,0.00044163558,0.018769285,0.0015668783,0.0014697466,0.00087257876,0.000027962156],"about_ca_topic_score_codex":0.0038810868,"about_ca_topic_score_gemma":0.0025277596,"teacher_disagreement_score":0.004261811,"about_ca_system_score_codex":0.00035909505,"about_ca_system_score_gemma":0.00031636027,"threshold_uncertainty_score":0.02253884},"labels":[],"label_agreement":null},{"id":"W2275220518","doi":"10.3847/0004-637x/820/2/137","title":"MODELING SEVEN YEARS OF EVENT HORIZON TELESCOPE OBSERVATIONS WITH RADIATIVELY INEFFICIENT ACCRETION FLOW MODELS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo","funders":"","keywords":"Context (archaeology); Magnitude (astronomy); Event horizon; Line-of-sight; Accretion (finance); Horizon; Event (particle physics); Position angle; Interferometry","score_opus":0.022613313318658974,"score_gpt":0.22845050110378445,"score_spread":0.20583718778512547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2275220518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922661,0.00013193136,0.004056882,0.00038474912,0.000025642274,0.00002774138,0.0009947465,0.00014565696,0.0019664702],"genre_scores_gemma":[0.99784434,0.000050028306,0.0008506665,0.000038517603,0.000016228947,0.000018514711,0.0007261701,0.00003001929,0.00042562908],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99969983,0.00008103314,0.00001759446,0.00009367157,0.000038727514,0.0000691311],"domain_scores_gemma":[0.9981731,0.00083690084,0.00035682102,0.00019324655,0.00016587524,0.00027397202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020740742,0.00049442175,0.0006195398,0.000714528,0.00073451054,0.0013138534,0.0018068615,0.0015156029,0.001866004],"category_scores_gemma":[0.0037631714,0.0005940984,0.0011661013,0.0007608794,0.0010521169,0.0012506198,0.0008115415,0.0011793312,0.0002799517],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033365432,0.0003136641,0.102389716,0.000047586334,0.00026145042,0.00049333606,0.00026654912,0.8815749,0.0013671812,0.007410624,0.0017790247,0.0037622468],"study_design_scores_gemma":[0.00005312723,0.000044218683,0.016079308,0.0000072607627,0.000045124845,0.000023401044,0.000049272992,0.9817618,0.00022606988,0.0011781392,0.00050729426,0.000024984225],"about_ca_topic_score_codex":0.05745555,"about_ca_topic_score_gemma":0.030160673,"teacher_disagreement_score":0.05745555,"about_ca_system_score_codex":0.0026820186,"about_ca_system_score_gemma":0.0007115622,"threshold_uncertainty_score":0.114242196},"labels":[],"label_agreement":null},{"id":"W2275280772","doi":"10.3847/0004-637x/824/2/84","title":"SUBMILLIMETER POLARIZATION SPECTRUM IN THE VELA C MOLECULAR CLOUD","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Office of Polar Programs; Science and Technology Facilities Council; Canadian Space Agency; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Leverhulme Trust; Ontario Innovation Trust; Illinois Space Grant Consortium; National Aeronautics and Space Administration; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"Vela; Physics; Astrophysics; Molecular cloud; Polarization (electrochemistry); Radiative transfer; Telescope; Polarimeter; Interstellar cloud; Planck; Cosmic dust; Astronomy; Optics; Pulsar; Stars; Scattering; Polarimetry","score_opus":0.006750251950228883,"score_gpt":0.21782243357965253,"score_spread":0.21107218162942365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2275280772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973761,0.000050962255,0.0001516891,0.00002669624,0.000003477862,0.0000033816589,0.0009193402,0.000020696887,0.0014476866],"genre_scores_gemma":[0.9987804,0.00002449274,0.00011128181,0.000009794112,0.000004385238,0.0000032565333,0.0008978899,0.000004504283,0.00016389799],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992883,0.000003952079,0.0000015803487,0.000020178617,0.000018272836,0.00002719777],"domain_scores_gemma":[0.9998035,0.0000373555,0.000042151918,0.000016637996,0.000050234972,0.000050218354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011179361,0.00012520504,0.00014909786,0.00087776146,0.0004063412,0.0004508389,0.00017894058,0.000188825,0.0010049437],"category_scores_gemma":[0.00025364995,0.00011347456,0.00012328461,0.00063302345,0.00013693969,0.000149755,0.00026702392,0.00029476034,0.00013655555],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064601406,0.00021803255,0.6836397,0.00006402019,0.00012981566,0.0006711893,0.0006253953,0.004144128,0.28555644,0.00085710577,0.0029956454,0.020452514],"study_design_scores_gemma":[0.000005950049,0.000014285246,0.99509794,0.000004571616,0.0000068869367,0.000045993525,0.00004840907,0.0015416896,0.002704653,0.000045369852,0.0004782709,0.0000059596177],"about_ca_topic_score_codex":0.009381691,"about_ca_topic_score_gemma":0.010340115,"teacher_disagreement_score":0.009381691,"about_ca_system_score_codex":0.00039668978,"about_ca_system_score_gemma":0.00013617391,"threshold_uncertainty_score":0.018654168},"labels":[],"label_agreement":null},{"id":"W2275691994","doi":"10.3847/0004-637x/819/2/155","title":"THE NANOGRAV NINE-YEAR DATA SET: NOISE BUDGET FOR PULSAR ARRIVAL TIMES ON INTRADAY TIMESCALES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"","keywords":"Physics; Pulsar; Noise (video); Astronomy; Astrophysics; Data set; Set (abstract data type); Statistics","score_opus":0.021923424163220902,"score_gpt":0.32893904677201746,"score_spread":0.30701562260879656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2275691994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9690607,0.00018747785,0.0073957616,0.00022036865,0.000033842745,0.000034513825,0.021019334,0.00029553648,0.0017524726],"genre_scores_gemma":[0.9517041,0.00007081892,0.0047747875,0.000059522725,0.000035967434,0.000064888496,0.042694084,0.00013877272,0.0004570767],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989354,0.00018665449,0.000145479,0.0003303818,0.00032024723,0.00008178785],"domain_scores_gemma":[0.9934902,0.0024130058,0.0011644483,0.0016572021,0.0010534844,0.00022166163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023774349,0.0002880138,0.00051183644,0.0022467854,0.0005188415,0.00091862807,0.0007845067,0.00049435295,0.0010131235],"category_scores_gemma":[0.007561487,0.00019954868,0.00040153615,0.0029743835,0.0003061082,0.00080075214,0.0007685082,0.00044670672,0.00046039606],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048478192,0.00010835593,0.93777305,0.000100059966,0.00033573268,0.00018587019,0.0002772026,0.015849002,0.011648,0.00085799076,0.004708846,0.027670998],"study_design_scores_gemma":[0.00002898196,0.00004815831,0.9624167,0.000015958476,0.000066136774,0.00020651812,0.00010733666,0.026916163,0.0046687876,0.00041396436,0.0050805905,0.000030702533],"about_ca_topic_score_codex":0.010767366,"about_ca_topic_score_gemma":0.012742554,"teacher_disagreement_score":0.010767366,"about_ca_system_score_codex":0.0004594064,"about_ca_system_score_gemma":0.00037552326,"threshold_uncertainty_score":0.021409392},"labels":[],"label_agreement":null},{"id":"W2276745816","doi":"10.1088/0004-637x/809/1/63","title":"MODELING ATMOSPHERIC EMISSION FOR CMB GROUND-BASED OBSERVATIONS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Cosmic microwave background; Atmosphere (unit); Atmospheric model; Physics; Meteorology; Wind speed; Environmental science; Parametric statistics; Noise (video); Computational physics; Remote sensing; Optics; Geology; Computer science; Statistics; Mathematics","score_opus":0.04478067805028798,"score_gpt":0.2587150928972624,"score_spread":0.21393441484697442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2276745816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91673934,0.0010944358,0.055736355,0.0019032676,0.00036077583,0.00008107843,0.0078088124,0.0027835653,0.013492405],"genre_scores_gemma":[0.98144275,0.00031271967,0.01117137,0.000084846506,0.00008811902,0.000049000177,0.0031126027,0.00020299321,0.003535706],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998584,0.000039772673,0.0000049609016,0.000048369904,0.00002354705,0.000024909523],"domain_scores_gemma":[0.9998012,0.000087885455,0.00002078809,0.000018661924,0.000041268904,0.000030323463],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032013556,0.0005430717,0.00031163442,0.0003865755,0.00047967111,0.0007854507,0.00089225714,0.0011463009,0.0017686641],"category_scores_gemma":[0.00081417,0.0003904968,0.0007821199,0.0008465153,0.00019594972,0.000716331,0.00037002712,0.0007475691,0.00039348236],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009934632,0.00010434904,0.013298319,0.000040957304,0.00012841262,0.00007052433,0.000049865463,0.9717029,0.0017075485,0.0018363015,0.00223133,0.008730192],"study_design_scores_gemma":[0.000040633986,0.000012090764,0.0038450728,0.000004849373,0.000019814797,0.000007890671,0.00002035752,0.99373406,0.00031362506,0.00072128297,0.0012680019,0.000012311244],"about_ca_topic_score_codex":0.14614956,"about_ca_topic_score_gemma":0.09313356,"teacher_disagreement_score":0.14614956,"about_ca_system_score_codex":0.0008551075,"about_ca_system_score_gemma":0.0015186121,"threshold_uncertainty_score":0.2905978},"labels":[],"label_agreement":null},{"id":"W2278589840","doi":"10.3847/0004-637x/819/1/24","title":"A SURVEY OF LUMINOUS HIGH-REDSHIFT QUASARS WITH SDSS AND WISE. I. TARGET SELECTION AND OPTICAL SPECTROSCOPY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astrophysik; People's Government of Yunnan Province; Chinese Academy of Sciences; York University; University of Cambridge; Pennsylvania State University; University of Virginia; Carnegie Mellon University; University of Arizona; College of Engineering, Michigan State University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; University of Utah; Harvard University; University of Florida; University of Tokyo; Ohio State University; National Natural Science Foundation of China; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Redshift; Quasar; Physics; Database; Analytical Chemistry (journal); Astrophysics; Algorithm; Materials science; Computer science; Chemistry; Galaxy","score_opus":0.0061245766640800345,"score_gpt":0.20509303214240227,"score_spread":0.19896845547832223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2278589840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957048,0.00025269084,0.00073333323,0.00005064286,0.0000072117255,0.000035665966,0.0023811604,0.000067071625,0.0007673438],"genre_scores_gemma":[0.98014736,0.0002875016,0.005641291,0.00012963286,0.000038206574,0.00004367474,0.012674223,0.000020056372,0.001018093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99948335,0.00007802392,0.00005318532,0.00011527328,0.00016905967,0.00010116525],"domain_scores_gemma":[0.99802893,0.00012152746,0.00074498926,0.00017344786,0.00032992742,0.0006011254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011932418,0.0004127039,0.00035173626,0.003040674,0.00037434677,0.00050706737,0.00040728546,0.00022912322,0.000618185],"category_scores_gemma":[0.00082527247,0.00029466988,0.00030171865,0.0018971357,0.00023076488,0.0003900866,0.00081254274,0.00022158852,0.00038928087],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008032764,0.00008992701,0.9686668,0.00006321178,0.000079440884,0.00014668336,0.00025443974,0.00011586436,0.01594224,0.00018193391,0.0012925388,0.0130866375],"study_design_scores_gemma":[0.000008338302,0.00004754695,0.9961391,0.0000044000903,0.000025253488,0.00014558999,0.000089377485,0.00031650648,0.0012365982,0.000019328094,0.0019625532,0.000005385841],"about_ca_topic_score_codex":0.0056620124,"about_ca_topic_score_gemma":0.010431478,"teacher_disagreement_score":0.0056620124,"about_ca_system_score_codex":0.00029235426,"about_ca_system_score_gemma":0.0004599469,"threshold_uncertainty_score":0.011258125},"labels":[],"label_agreement":null},{"id":"W2278842478","doi":"10.3847/0004-637x/817/2/88","title":"A SEARCH FOR HYPERLUMINOUS X-RAY SOURCES IN THE XMM-NEWTON SOURCE CATALOG","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Galaxy; Sky; Redshift; Active galactic nucleus; Telescope; Star formation","score_opus":0.011179423087719674,"score_gpt":0.22381464805517523,"score_spread":0.21263522496745554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2278842478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.970991,0.00053326046,0.010667162,0.00010737725,0.000013489456,0.0001663396,0.012586851,0.00092193816,0.004012485],"genre_scores_gemma":[0.9183597,0.00029344767,0.03143497,0.000101614845,0.000082564475,0.00021558297,0.045860864,0.00007906281,0.0035722782],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994715,0.000041192623,0.000065835105,0.00012651055,0.00022881813,0.00006616757],"domain_scores_gemma":[0.9976927,0.00042602388,0.0007867482,0.0005249737,0.00032051696,0.00024899901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010932231,0.0003025459,0.0003090335,0.010131225,0.000497928,0.0011376175,0.0006818947,0.00043507715,0.0066689095],"category_scores_gemma":[0.0020453327,0.00018532592,0.00023111652,0.0038215434,0.00016157815,0.0006061768,0.0011497505,0.00021598318,0.0026035036],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020206432,0.00014957659,0.90917516,0.000085281456,0.00008140058,0.0005286671,0.0002780163,0.0006572965,0.013063646,0.0010623146,0.003494638,0.071221955],"study_design_scores_gemma":[0.000034054894,0.00005946766,0.9756842,0.00004024528,0.000064695014,0.00063717493,0.00014554046,0.008172682,0.004614622,0.00038817825,0.0101405475,0.000018566303],"about_ca_topic_score_codex":0.002800172,"about_ca_topic_score_gemma":0.004668303,"teacher_disagreement_score":0.010131225,"about_ca_system_score_codex":0.00027091947,"about_ca_system_score_gemma":0.000545028,"threshold_uncertainty_score":0.02230966},"labels":[],"label_agreement":null},{"id":"W2280035439","doi":"10.3847/0004-637x/821/1/27","title":"CONSTRAINING WHITE DWARF STRUCTURE AND NEUTRINO PHYSICS IN 47 TUCANAE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"White dwarf; Physics; Astrophysics; Neutrino; Markov chain Monte Carlo; Stars; Monte Carlo method; Hubble space telescope; Astronomy; Particle physics; Statistics","score_opus":0.014169185111891087,"score_gpt":0.22670267021567095,"score_spread":0.21253348510377987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2280035439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996411,0.00009294606,0.0017359005,0.00004277694,0.0000037195016,0.0000066359667,0.0008635146,0.000087039385,0.00075646845],"genre_scores_gemma":[0.9965636,0.000027091119,0.0011723705,0.000013860259,0.0000048639145,0.000010797737,0.001892481,0.00003931744,0.00027559174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965143,0.000035078545,0.000011472993,0.00010638452,0.00008977992,0.000105912884],"domain_scores_gemma":[0.9990491,0.0002516111,0.0001825731,0.00012249385,0.00025639366,0.00013777714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00073694525,0.00035246718,0.0006649715,0.0023304194,0.0019614983,0.001103673,0.00100047,0.00051717064,0.0014226611],"category_scores_gemma":[0.0022482867,0.00027637862,0.0006365933,0.0023271965,0.00077991845,0.00022471826,0.0006897026,0.0003941119,0.00023236647],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003281496,0.000058577283,0.8917842,0.00003774899,0.00036294904,0.00020211852,0.0003413967,0.059739403,0.020318238,0.0018192731,0.0012158987,0.023792159],"study_design_scores_gemma":[0.00001826037,0.000025720889,0.9227694,0.000011503466,0.000068006164,0.000046672154,0.00030947287,0.06921772,0.0035134736,0.0007666481,0.0032103013,0.000042797503],"about_ca_topic_score_codex":0.46990496,"about_ca_topic_score_gemma":0.41593155,"teacher_disagreement_score":0.46990496,"about_ca_system_score_codex":0.0027760735,"about_ca_system_score_gemma":0.0024238036,"threshold_uncertainty_score":0.93433964},"labels":[],"label_agreement":null},{"id":"W2280809684","doi":"10.3847/0004-637x/821/2/109","title":"ON THE LAUNCHING AND STRUCTURE OF RADIATIVELY DRIVEN WINDS IN WOLF–RAYET STARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Hydrostatic equilibrium; Stars; Opacity; Radiation pressure; Supersonic speed; Radiative transfer; Convection; Outflow; Stellar wind","score_opus":0.007380400101568226,"score_gpt":0.2088415700427914,"score_spread":0.20146116994122318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2280809684","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99887305,0.000026343698,0.00022270878,0.000018302682,0.0000019315369,0.0000024741914,0.00002620336,0.0000124510525,0.000816562],"genre_scores_gemma":[0.9994758,0.00001169332,0.0001565616,0.0000052260457,0.0000032292617,0.0000017092383,0.00006932672,0.000006536228,0.00027001413],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995494,0.000008017635,0.0000031535671,0.0000097954035,0.000008662619,0.000015476875],"domain_scores_gemma":[0.9994311,0.000093896975,0.00016264716,0.000027183973,0.00008078808,0.00020441442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021396404,0.00021150871,0.0002269278,0.00064024836,0.00045741184,0.00096411066,0.00026979484,0.00043621834,0.0012386462],"category_scores_gemma":[0.00079747237,0.00022430449,0.0001857188,0.00025777676,0.0004816532,0.00035670836,0.00075701624,0.00036674054,0.0003009777],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010786124,0.0005963262,0.7715619,0.00007163811,0.0001390241,0.0023813772,0.0012179007,0.07528636,0.10750369,0.015243699,0.0013547253,0.023564802],"study_design_scores_gemma":[0.000096268086,0.00042799607,0.8033566,0.00004189157,0.000027117741,0.0004311857,0.0008518507,0.1796042,0.007598062,0.0058824974,0.0016249486,0.000057307392],"about_ca_topic_score_codex":0.001468047,"about_ca_topic_score_gemma":0.0014112816,"teacher_disagreement_score":0.001468047,"about_ca_system_score_codex":0.0004692495,"about_ca_system_score_gemma":0.00016097871,"threshold_uncertainty_score":0.0041436553},"labels":[],"label_agreement":null},{"id":"W2281136567","doi":"10.3847/0004-637x/820/2/90","title":"PERSISTENT ASYMMETRIC STRUCTURE OF SAGITTARIUS A* ON EVENT HORIZON SCALES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Japan Society for the Promotion of Science; Science and Technology Facilities Council; Army Research Office; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Industry Canada; Academia Sinica; National Science Foundation; Government of Canada; Smithsonian Astrophysical Observatory; Gordon and Betty Moore Foundation; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Sagittarius A*; Physics; Astrophysics; Galactic Center; Event horizon; Asymmetry; Schwarzschild radius; Astronomy; Amplitude; Millimeter; Angular resolution (graph drawing); Extinction (optical mineralogy); Supermassive black hole; Event (particle physics); Galaxy; Optics; Accretion (finance)","score_opus":0.009940024106000452,"score_gpt":0.22310787472997048,"score_spread":0.21316785062397003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2281136567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986771,0.000042108764,0.00015793597,0.000015843643,0.0000023094071,0.000002777957,0.00028659447,0.000024027588,0.0007912807],"genre_scores_gemma":[0.9990018,0.000013736396,0.000088751076,0.000004557215,0.000004378587,0.0000024508697,0.00079314446,0.0000071331824,0.000084132065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988544,0.0000130941435,0.000008160946,0.000031469626,0.000033315413,0.000028483739],"domain_scores_gemma":[0.999164,0.000079161815,0.0002949105,0.00009606308,0.0001546889,0.00021112815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019752486,0.00013918224,0.0003104758,0.0014870422,0.00042389668,0.0005977203,0.0002637785,0.00017357376,0.00085304456],"category_scores_gemma":[0.0006814737,0.000119052296,0.0001878012,0.0008973757,0.0003584139,0.00029603895,0.00060974795,0.00025071544,0.0002168271],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006940954,0.0001680339,0.814042,0.000045221223,0.0001553046,0.00047888263,0.0008143031,0.0015143047,0.15908842,0.0007097941,0.0010764676,0.02121317],"study_design_scores_gemma":[0.0000031107882,0.000036262045,0.99785763,0.0000015356841,0.0000046474183,0.000050762177,0.0000818666,0.0005958973,0.0008719431,0.000075472366,0.00041660786,0.0000043535183],"about_ca_topic_score_codex":0.009408518,"about_ca_topic_score_gemma":0.008881284,"teacher_disagreement_score":0.009408518,"about_ca_system_score_codex":0.00043669244,"about_ca_system_score_gemma":0.00017403382,"threshold_uncertainty_score":0.018707454},"labels":[],"label_agreement":null},{"id":"W2281497325","doi":"10.3847/0004-637x/817/1/29","title":"PHOTOIONIZATION MODELS OF THE INNER GASEOUS DISK OF THE HERBIG BE STAR BD+65 1637","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Western University","funders":"","keywords":"Be star; Line (geometry); Spectral line; Emission spectrum; Photoionization; Herbig Ae/Be star; Thick disk; Electron density; Thin disk","score_opus":0.011269862461471832,"score_gpt":0.21240376927666196,"score_spread":0.20113390681519014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2281497325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99608326,0.00008359239,0.001721545,0.000030507985,0.0000021330088,0.0000070717215,0.00007726765,0.000025243933,0.001969322],"genre_scores_gemma":[0.9993286,0.0000327858,0.0002681722,0.00001117977,0.0000012366164,0.000004900895,0.00009360841,0.0000064400724,0.00025317405],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999591,0.000006621605,0.0000021237859,0.00001090273,0.000009209852,0.000012093706],"domain_scores_gemma":[0.99989927,0.000023360417,0.000025269934,0.000010998927,0.0000138888645,0.00002715006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011410988,0.00033957022,0.00028090883,0.0002908788,0.00039236966,0.0004825746,0.0006824746,0.0005284242,0.0009300369],"category_scores_gemma":[0.00028371587,0.00021670807,0.00032162815,0.0002207829,0.00030477566,0.0003395636,0.0002625598,0.00015305134,0.00026920054],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005881529,0.00024524433,0.19248655,0.00013912447,0.00016794392,0.0014992908,0.0005853068,0.6616867,0.12481171,0.007187673,0.0007120306,0.009890315],"study_design_scores_gemma":[0.000107903914,0.00018693728,0.08814851,0.000020026113,0.000047009944,0.00017650372,0.00030419667,0.9019255,0.0056836247,0.002057555,0.0013130836,0.000029136658],"about_ca_topic_score_codex":0.012833344,"about_ca_topic_score_gemma":0.005854702,"teacher_disagreement_score":0.012833344,"about_ca_system_score_codex":0.0010181624,"about_ca_system_score_gemma":0.00020839155,"threshold_uncertainty_score":0.025517344},"labels":[],"label_agreement":null},{"id":"W2281864350","doi":"10.3847/0004-637x/820/2/139","title":"STABLE AND UNSTABLE REGIMES OF MASS ACCRETION ONTO RW AUR A","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; T Tauri star; Photometry (optics); Accretion (finance); Redshift; Astronomy; Spectral line; Occultation; Stars; Galaxy","score_opus":0.008998983483875723,"score_gpt":0.2241234468336475,"score_spread":0.21512446334977176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2281864350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983536,0.00012468854,0.00007842669,0.000019976665,0.0000030084875,0.0000026497473,0.00012651013,0.000015058787,0.0012761314],"genre_scores_gemma":[0.9996822,0.000036145637,0.00005077833,0.000005348016,0.0000068544337,0.0000013455231,0.00012568367,0.0000020235714,0.00008956776],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981576,0.00002025227,0.00001568837,0.000060179143,0.000035112524,0.000052879775],"domain_scores_gemma":[0.99952114,0.000048404985,0.0002222147,0.000043103766,0.000065236614,0.00009980978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024160108,0.00021561242,0.00026398804,0.0010423696,0.00047143633,0.0007917341,0.00036235113,0.00023733256,0.00070992135],"category_scores_gemma":[0.0006816978,0.00013618065,0.00020746292,0.00042573118,0.00040723252,0.00040300642,0.00066730747,0.00021502524,0.00028321563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003407257,0.00005143909,0.96397555,0.000042392614,0.00010002959,0.00062797405,0.00030692155,0.000451622,0.025420256,0.0002339829,0.0002982322,0.008150843],"study_design_scores_gemma":[0.0000036232236,0.000041422834,0.9972452,0.0000066101047,0.0000146590055,0.00018700036,0.00013456872,0.0006684516,0.0011483651,0.000068628266,0.00047698195,0.0000045039355],"about_ca_topic_score_codex":0.0038093205,"about_ca_topic_score_gemma":0.0046855435,"teacher_disagreement_score":0.0038093205,"about_ca_system_score_codex":0.00041325836,"about_ca_system_score_gemma":0.00016713353,"threshold_uncertainty_score":0.00757432},"labels":[],"label_agreement":null},{"id":"W2283007205","doi":"10.3847/0004-637x/819/2/124","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. XIX. TOMOGRAPHY OF MILKY WAY SUBSTRUCTURES IN THE NGVS FOOTPRINT","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Milky Way; Sagittarius; Virgo Cluster; Sky; Star cluster; Galactic halo; Halo; Galaxy","score_opus":0.03253063000440778,"score_gpt":0.2745923893304881,"score_spread":0.2420617593260803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2283007205","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9764015,0.00047852387,0.0015929195,0.00011738267,0.000007282421,0.000031706004,0.013491319,0.00045716314,0.0074220756],"genre_scores_gemma":[0.9790469,0.00013467851,0.0033794544,0.000046845704,0.00001261411,0.000020009125,0.015818624,0.00006922211,0.0014716734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987507,0.000016324595,0.0000047414396,0.000028563907,0.000044023556,0.00003125232],"domain_scores_gemma":[0.9996395,0.000035221798,0.00012167517,0.00007529772,0.000049987422,0.00007836844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022543743,0.00018896133,0.00011983831,0.001452526,0.0001770685,0.00045493414,0.00028915895,0.00019732119,0.0022665747],"category_scores_gemma":[0.0004679503,0.00012851306,0.0002026984,0.0013019001,0.00012994159,0.0002462535,0.00060858444,0.00013445425,0.0008955427],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010603381,0.000025758549,0.95368266,0.000042994117,0.00007133949,0.00019952605,0.0002514997,0.0034741263,0.009083835,0.00037592213,0.0045731138,0.028113218],"study_design_scores_gemma":[0.0000056771705,0.000008411417,0.99356467,0.000007812791,0.0000075982557,0.00007047806,0.0001077774,0.0020324779,0.0007006654,0.000131652,0.003358649,0.000004092651],"about_ca_topic_score_codex":0.025856547,"about_ca_topic_score_gemma":0.04873584,"teacher_disagreement_score":0.025856547,"about_ca_system_score_codex":0.00043544997,"about_ca_system_score_gemma":0.00022365592,"threshold_uncertainty_score":0.051412106},"labels":[],"label_agreement":null},{"id":"W2284752184","doi":"10.1088/0004-637x/787/2/112","title":"<i>HERSCHEL</i>OBSERVATIONS OF EXTRAORDINARY SOURCES: ANALYSIS OF THE HIFI 1.2 THz WIDE SPECTRAL SURVEY TOWARD ORION KL. I. METHODS","year":2014,"lang":"no","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Terahertz radiation; Astronomy; Astrophysics; Optics","score_opus":0.04356955428298698,"score_gpt":0.30112915231648885,"score_spread":0.25755959803350187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2284752184","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92861396,0.00095091,0.0061307894,0.00029414572,0.000016235153,0.00012111868,0.056150824,0.0009295839,0.0067924005],"genre_scores_gemma":[0.8773575,0.00073240505,0.026729105,0.00030412027,0.000095232965,0.00024133988,0.092301115,0.00021846911,0.0020206275],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9997695,0.000025164094,0.000010449547,0.000059140446,0.00007050193,0.000065126245],"domain_scores_gemma":[0.99963605,0.000038080227,0.00017200063,0.000073705225,0.000027629785,0.000052559284],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033951728,0.00038625632,0.00014620958,0.0020994192,0.00034914026,0.0003960859,0.00042162594,0.00025132886,0.0018973968],"category_scores_gemma":[0.0003169877,0.00014598154,0.0003618159,0.0013632001,0.00018666059,0.00020153997,0.0005199183,0.00021831864,0.00079412403],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009278654,0.00016145094,0.85983115,0.00022528657,0.00022783567,0.00040992748,0.00031309098,0.009978277,0.055939253,0.00168651,0.017049324,0.054085065],"study_design_scores_gemma":[0.000013730437,0.000025906878,0.9743386,0.0000171376,0.000037999493,0.0002696983,0.000085093925,0.0038995973,0.0040442417,0.00027298048,0.016972275,0.000022739534],"about_ca_topic_score_codex":0.008521337,"about_ca_topic_score_gemma":0.014008428,"teacher_disagreement_score":0.008521337,"about_ca_system_score_codex":0.0005605179,"about_ca_system_score_gemma":0.0003135196,"threshold_uncertainty_score":0.016943514},"labels":[],"label_agreement":null},{"id":"W2286172744","doi":"10.3847/0004-637x/822/2/113","title":"VUV PHOTO-PROCESSING OF PAH CATIONS: QUANTITATIVE STUDY ON THE IONIZATION VERSUS FRAGMENTATION PROCESSES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Ottawa","funders":"","keywords":"Ionization; Fragmentation (computing); Photoionization; Photodissociation; Photon; Spectroscopy; Interstellar medium; Electron ionization; Ion","score_opus":0.03686706353800736,"score_gpt":0.3088061363989073,"score_spread":0.27193907286089997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2286172744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9851246,0.0019188817,0.009487407,0.000057635003,0.000015955377,0.00003775386,0.00036229158,0.00008747459,0.002907976],"genre_scores_gemma":[0.9935235,0.00070142763,0.0041082604,0.00005018488,0.000009496086,0.00003305044,0.00031792256,0.000023575167,0.0012325323],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998024,0.000024977206,0.0000048601555,0.00005934528,0.000059752238,0.00004874469],"domain_scores_gemma":[0.999721,0.00012833181,0.000054348384,0.000019855739,0.000053265583,0.000023159888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027139462,0.00041602665,0.00013912068,0.00050631224,0.00024349877,0.0003094191,0.00038436573,0.00057006924,0.0022201405],"category_scores_gemma":[0.0004598636,0.00017421812,0.00025295225,0.00035969925,0.00026530997,0.0004632684,0.00028244767,0.00050983595,0.0003515745],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020361463,0.00003880221,0.0053151953,0.00011442057,0.000026779027,0.000063898355,0.000085829866,0.0006012983,0.9864763,0.00029313378,0.00007840384,0.006702247],"study_design_scores_gemma":[0.000008520997,0.0002497173,0.030870007,0.000014678715,0.000026079697,0.00027359283,0.0001182884,0.0071632806,0.9593075,0.00024451513,0.0017091132,0.000014554128],"about_ca_topic_score_codex":0.00049571076,"about_ca_topic_score_gemma":0.00038649573,"teacher_disagreement_score":0.0022201405,"about_ca_system_score_codex":0.0002455642,"about_ca_system_score_gemma":0.00010602794,"threshold_uncertainty_score":0.007427156},"labels":[],"label_agreement":null},{"id":"W2287330447","doi":"10.1088/0004-637x/764/2/137","title":"CONSTRAINTS ON PERTURBATIONS TO THE RECOMBINATION HISTORY FROM MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND DAMPING TAIL","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Planck; Recombination; Ionization; Cosmic background radiation; Cosmology; Helium","score_opus":0.03020228106946611,"score_gpt":0.24174036334107263,"score_spread":0.21153808227160653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2287330447","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96801525,0.00030809196,0.023010291,0.00030720944,0.000024193061,0.00001229283,0.0024385694,0.00023683744,0.005647314],"genre_scores_gemma":[0.99460596,0.00011816598,0.0025381476,0.000037136295,0.000020421914,0.0000082385,0.0024167122,0.000072237,0.00018296878],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995672,0.00015243133,0.000026325728,0.00012622654,0.00007079074,0.000057060985],"domain_scores_gemma":[0.99716336,0.001169829,0.00056997966,0.0007315519,0.00015163883,0.00021354994],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002006245,0.0005484941,0.00024524808,0.0007384964,0.0003202064,0.0010924559,0.00041319575,0.00042120976,0.0016107728],"category_scores_gemma":[0.007409275,0.00031780527,0.0005376734,0.0007500977,0.0005340422,0.0009964909,0.00095628295,0.0008185913,0.00034355832],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010070608,0.00008492299,0.781086,0.00034791735,0.0006353609,0.00038128108,0.0007870469,0.07093079,0.061939932,0.027394492,0.004324601,0.051080458],"study_design_scores_gemma":[0.00007745647,0.00006374349,0.8406315,0.00009912268,0.00012323799,0.0002254515,0.00019363443,0.12403035,0.013119743,0.011469037,0.009881414,0.00008528634],"about_ca_topic_score_codex":0.0037708678,"about_ca_topic_score_gemma":0.0043248483,"teacher_disagreement_score":0.0037708678,"about_ca_system_score_codex":0.00031359072,"about_ca_system_score_gemma":0.00040293997,"threshold_uncertainty_score":0.010610163},"labels":[],"label_agreement":null},{"id":"W2287429402","doi":"10.3847/0004-637x/818/2/166","title":"THE NANOGRAV NINE-YEAR DATA SET: MONITORING INTERSTELLAR SCATTERING DELAYS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"","keywords":"Pulsar; Scintillation; Physics; Scattering; Astrophysics; Interstellar medium; Telescope; Green Bank Telescope; Scaling; Time of arrival; Computational physics; Optics; Detector; Galaxy","score_opus":0.03318525018242059,"score_gpt":0.3375550190958837,"score_spread":0.3043697689134631,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2287429402","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96429616,0.00016650723,0.0025052016,0.00011045127,0.000045845245,0.000043300184,0.029771987,0.00026051863,0.0028000246],"genre_scores_gemma":[0.9042889,0.00014617512,0.007526786,0.00007410564,0.000058077054,0.00009636152,0.08664411,0.000084344145,0.0010811583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996314,0.00004972238,0.00003355986,0.00010149142,0.00014927679,0.000034473265],"domain_scores_gemma":[0.9983902,0.00024171722,0.0003723181,0.0003987315,0.00041288394,0.00018426075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008582289,0.0002742917,0.00031930525,0.0016828857,0.00040755214,0.0005126389,0.00047423659,0.00033231868,0.000824532],"category_scores_gemma":[0.0013518597,0.00013075421,0.000215836,0.0015481005,0.00019413502,0.0005096819,0.0006049449,0.0003773189,0.00050043105],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009893065,0.000399014,0.8828078,0.00017411396,0.00030556333,0.00057244214,0.0004584661,0.011985882,0.03192894,0.0010400653,0.013511833,0.055826697],"study_design_scores_gemma":[0.000065800676,0.00015074642,0.9570274,0.00001413888,0.000055398836,0.00025585497,0.00014910061,0.013677233,0.009390435,0.00026924274,0.01890932,0.00003546675],"about_ca_topic_score_codex":0.009561237,"about_ca_topic_score_gemma":0.024494449,"teacher_disagreement_score":0.009561237,"about_ca_system_score_codex":0.00033337378,"about_ca_system_score_gemma":0.0003727416,"threshold_uncertainty_score":0.0190112},"labels":[],"label_agreement":null},{"id":"W2287838863","doi":"10.1088/0004-637x/805/2/141","title":"HIGH-RESOLUTION FOURIER-TRANSFORM MICROWAVE SPECTROSCOPY OF METHYL- AND DIMETHYLNAPTHALENES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Molecular Spectroscopy and Structure","field":"Chemistry","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Rotational spectroscopy; Spectral line; Microwave; Fourier transform spectroscopy; Spectroscopy; Fourier transform; Physics; Rotational transition; Fourier transform infrared spectroscopy; Resolution (logic); Cosmic microwave background; Polar; Analytical Chemistry (journal); Chemistry; Optics; Astronomy; Organic chemistry","score_opus":0.008917976688775657,"score_gpt":0.23923523834458138,"score_spread":0.2303172616558057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2287838863","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99160683,0.0007747208,0.005262789,0.000045237073,0.0000099783865,0.000008308093,0.00040911755,0.000030131056,0.0018529212],"genre_scores_gemma":[0.9920604,0.0006369942,0.005314529,0.000024517352,0.000007965382,0.000011618678,0.0005427883,0.00001066434,0.0013905076],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998834,0.000015593754,0.000004273255,0.000021603255,0.000054006257,0.000021142601],"domain_scores_gemma":[0.9998926,0.000039737144,0.000023115226,0.000009105595,0.000024828361,0.000010627159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023845508,0.00026622164,0.00014123428,0.00032013372,0.00014902437,0.00010440162,0.0003248915,0.00019626871,0.0013892414],"category_scores_gemma":[0.00022782641,0.00013832278,0.00011729903,0.00025538867,0.00013346506,0.0002774886,0.00014907838,0.00031492786,0.000158062],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007976136,0.000014397734,0.0006403293,0.00003654452,0.000006493895,0.000039071092,0.000037369857,0.00028183253,0.9963225,0.00023942254,0.00005077746,0.002251462],"study_design_scores_gemma":[0.000012711161,0.00016166795,0.010966127,0.000007540233,0.000012066922,0.00014818036,0.000057195506,0.005458956,0.98131895,0.00013452928,0.0017082958,0.000013689819],"about_ca_topic_score_codex":0.00069276016,"about_ca_topic_score_gemma":0.0012756761,"teacher_disagreement_score":0.0013892414,"about_ca_system_score_codex":0.00014405216,"about_ca_system_score_gemma":0.000075941905,"threshold_uncertainty_score":0.0046474338},"labels":[],"label_agreement":null},{"id":"W2288417487","doi":"10.3847/0004-637x/818/2/194","title":"DISPERSAL OF TIDAL DEBRIS IN A MILKY-WAY-SIZED DARK MATTER HALO","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Halo; Physics; Astrophysics; Dark matter; Dark matter halo; Globular cluster; Galaxy; Milky Way; Astronomy; Cuspy halo problem","score_opus":0.005457158045853871,"score_gpt":0.2035499151205643,"score_spread":0.19809275707471044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2288417487","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99793696,0.000048123693,0.000523434,0.000090594855,0.000007769594,0.000010653066,0.00017138485,0.00003879743,0.001172242],"genre_scores_gemma":[0.99880004,0.000036872865,0.000510419,0.000029483526,0.0000035245741,0.000008599291,0.00020000311,0.000011784748,0.00039905173],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990237,0.000029133855,0.000004262225,0.000012816799,0.000011321718,0.00004005695],"domain_scores_gemma":[0.99927443,0.00024025905,0.000074131116,0.0000671096,0.00008401886,0.000260168],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040308404,0.0003556747,0.00040611098,0.0005814429,0.00056537293,0.00085990253,0.0008883914,0.00068149803,0.001612946],"category_scores_gemma":[0.0019414084,0.00024243661,0.0005851109,0.00046482074,0.0009916518,0.0005268383,0.0011361944,0.0005137714,0.00013213973],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032275188,0.00012751378,0.04196809,0.00003227837,0.000092701026,0.00034248218,0.00016363696,0.95064527,0.001628236,0.002614197,0.00053544744,0.0015273843],"study_design_scores_gemma":[0.00026604978,0.00018662828,0.014441052,0.00001725543,0.00004876621,0.000049672584,0.00033460208,0.98192143,0.000710906,0.0013839289,0.0006139238,0.000025682972],"about_ca_topic_score_codex":0.043346882,"about_ca_topic_score_gemma":0.02093906,"teacher_disagreement_score":0.043346882,"about_ca_system_score_codex":0.0011745129,"about_ca_system_score_gemma":0.0008337708,"threshold_uncertainty_score":0.08618915},"labels":[],"label_agreement":null},{"id":"W2288641441","doi":"10.3847/0004-637x/819/2/147","title":"THE ISLANDS PROJECT. I. ANDROMEDA XVI, AN EXTREMELY LOW MASS GALAXY NOT QUENCHED BY REIONIZATION*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Andromeda; Star formation; Andromeda Galaxy; Galaxy; Reionization; Stars; Globular cluster; Local Group","score_opus":0.011702409062553796,"score_gpt":0.24043773459433904,"score_spread":0.22873532553178524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2288641441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91969836,0.003732498,0.00086304464,0.00096380187,0.00005833143,0.00015372345,0.04100155,0.0003222426,0.03320655],"genre_scores_gemma":[0.9428357,0.0009860654,0.0039658872,0.00015702996,0.00007181728,0.000096853575,0.036566034,0.000109003675,0.015211574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998528,0.000028282077,0.0000048679294,0.000047665533,0.000034382618,0.000032033306],"domain_scores_gemma":[0.99941385,0.000038504273,0.00012858034,0.000082558516,0.000090410125,0.0002461108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031315006,0.0002616412,0.00017553371,0.0007194456,0.00025490313,0.00047169862,0.00033193652,0.00012593243,0.003346633],"category_scores_gemma":[0.0004262867,0.000080016325,0.00014547781,0.00047998028,0.00019071059,0.0001531826,0.0007728383,0.0001882544,0.00089378795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009045219,0.000091507725,0.85547376,0.00037650103,0.00018042592,0.0005217666,0.0006702108,0.00057426764,0.0116639305,0.0017087996,0.019678127,0.10815619],"study_design_scores_gemma":[0.00002773426,0.00006231818,0.96279526,0.000034150085,0.000050639923,0.00020261842,0.00021632995,0.00025109822,0.0009443579,0.000097968936,0.035311565,0.0000058895553],"about_ca_topic_score_codex":0.06484765,"about_ca_topic_score_gemma":0.09491668,"teacher_disagreement_score":0.06484765,"about_ca_system_score_codex":0.00054269214,"about_ca_system_score_gemma":0.0006818872,"threshold_uncertainty_score":0.1289404},"labels":[],"label_agreement":null},{"id":"W2288676749","doi":"10.3847/0004-637x/826/2/220","title":"ANISOTROPY IN COSMIC-RAY ARRIVAL DIRECTIONS IN THE SOUTHERN HEMISPHERE BASED ON SIX YEARS OF DATA FROM THE ICECUBE DETECTOR","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; University of Oxford; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Anisotropy; Muon; Cosmic ray; Angular resolution (graph drawing); Neutrino; Astrophysics; Amplitude; Multipole expansion; Observatory; Detector; Astronomy; Computational physics; Nuclear physics; Optics","score_opus":0.016139411801718243,"score_gpt":0.23657106305967562,"score_spread":0.22043165125795738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2288676749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9815291,0.00033821032,0.0004179685,0.00004652102,0.0000136141825,0.000011461525,0.015709765,0.000054337102,0.0018791605],"genre_scores_gemma":[0.96553534,0.00021452592,0.00046791707,0.000013464583,0.00002082786,0.000014075508,0.033500705,0.000026899585,0.00020614451],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994863,0.0001134973,0.000049780258,0.00013302299,0.00012947788,0.00008784782],"domain_scores_gemma":[0.99769443,0.00048335237,0.0008735949,0.000339321,0.00038499662,0.000224307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001364959,0.00041274598,0.00044000184,0.0019821066,0.0002558483,0.00085267995,0.00025833008,0.00028028607,0.00081039575],"category_scores_gemma":[0.0021995008,0.00021888642,0.00042491924,0.0020951629,0.00028535168,0.00036673743,0.0005195757,0.0002982378,0.00028015114],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046758508,0.000060112583,0.9808046,0.000051672145,0.00027759594,0.00024308942,0.00015485898,0.0065373275,0.003318859,0.00018677583,0.0015298238,0.0063677076],"study_design_scores_gemma":[0.000009038483,0.00002947811,0.99451363,0.0000094700445,0.000033245156,0.00012165745,0.000040550847,0.002590299,0.0008256755,0.000059311868,0.0017572312,0.000010396158],"about_ca_topic_score_codex":0.012686266,"about_ca_topic_score_gemma":0.018618943,"teacher_disagreement_score":0.012686266,"about_ca_system_score_codex":0.00058938545,"about_ca_system_score_gemma":0.0003721501,"threshold_uncertainty_score":0.025224805},"labels":[],"label_agreement":null},{"id":"W2289407240","doi":"10.3847/0004-637x/821/2/129","title":"TEV GAMMA-RAY OBSERVATIONS OF THE GALACTIC CENTER RIDGE BY VERITAS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Galactic Center; Astrophysics; Galactic plane; Gamma ray; Supermassive black hole; Astronomy; Galaxy; Supernova remnant; Telescope; Supernova; Ridge","score_opus":0.011489604432325677,"score_gpt":0.21083627975180322,"score_spread":0.19934667531947753,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2289407240","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98605114,0.00025379547,0.0006061799,0.000101050646,0.000019904373,0.00001243649,0.0034390246,0.00031899978,0.00919756],"genre_scores_gemma":[0.9887678,0.00013442725,0.0028370817,0.00007248328,0.000032454333,0.0000076017373,0.005817742,0.0000736812,0.002256723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997379,0.00001660693,0.000007795939,0.00007531461,0.00011362541,0.00004883255],"domain_scores_gemma":[0.9993875,0.00006820418,0.00017244494,0.00012832606,0.00014171198,0.00010185398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031640613,0.00020451589,0.00025734262,0.0010734316,0.00037867707,0.00057917624,0.00051609956,0.00021867135,0.0024013564],"category_scores_gemma":[0.0003986358,0.00023461203,0.0002858745,0.00069216394,0.00018262639,0.00028261333,0.000695833,0.00049076945,0.00057385885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012994402,0.00018747215,0.5593153,0.00006860321,0.00032175166,0.0010008336,0.0006754036,0.0017970768,0.3825028,0.0010149215,0.0071562827,0.044660125],"study_design_scores_gemma":[0.00005724109,0.00012879245,0.97851104,0.000019245012,0.00005527938,0.0003768962,0.00012691838,0.0019307166,0.010924492,0.00009989318,0.00775507,0.00001441397],"about_ca_topic_score_codex":0.026565129,"about_ca_topic_score_gemma":0.06170911,"teacher_disagreement_score":0.026565129,"about_ca_system_score_codex":0.0006567646,"about_ca_system_score_gemma":0.00037633462,"threshold_uncertainty_score":0.05282104},"labels":[],"label_agreement":null},{"id":"W2290090548","doi":"10.1088/0004-637x/767/2/148","title":"SATURATION OF THE MAGNETO-ROTATIONAL INSTABILITY IN STRONGLY RADIATION-DOMINATED ACCRETION DISKS","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Turbulence; Magnetohydrodynamics; Radiative transfer; Accretion (finance); Prandtl number; Saturation (graph theory); Instability; Magnetic Prandtl number; Reynolds stress; Viscosity","score_opus":0.0073721702338136064,"score_gpt":0.2291059321824277,"score_spread":0.22173376194861408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2290090548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99704164,0.0001078859,0.001493294,0.00003313561,0.000003606617,0.000005376642,0.000023729423,0.000061600644,0.0012298481],"genre_scores_gemma":[0.9994466,0.000026589336,0.00040452473,0.00000410889,0.0000025945008,0.000004009446,0.000015430123,0.000007673159,0.00008843271],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992156,0.000020292173,0.000006429664,0.000012881501,0.000017354714,0.000021399923],"domain_scores_gemma":[0.9994746,0.00020730555,0.00014711174,0.000045163706,0.00006120161,0.00006458146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015483849,0.00038567386,0.0002929804,0.00032292042,0.00028548174,0.00047757925,0.00044646068,0.00031028493,0.00040442866],"category_scores_gemma":[0.0011191592,0.00018076332,0.00026997007,0.00017099177,0.00045743847,0.00031474777,0.00068204256,0.0003520818,0.0001111714],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013613492,0.00026907367,0.075137615,0.00036355396,0.00014497867,0.002176885,0.0012105089,0.24901651,0.6429827,0.0072159916,0.0005931562,0.01952767],"study_design_scores_gemma":[0.00007758071,0.0002915291,0.027246175,0.0000227293,0.000018776593,0.00017429794,0.000103876766,0.90746486,0.06311984,0.0011533038,0.0003006912,0.000026338403],"about_ca_topic_score_codex":0.0011356852,"about_ca_topic_score_gemma":0.00046814975,"teacher_disagreement_score":0.0011356852,"about_ca_system_score_codex":0.00033108259,"about_ca_system_score_gemma":0.00023920787,"threshold_uncertainty_score":0.002402246},"labels":[],"label_agreement":null},{"id":"W2290284740","doi":"10.3847/0004-637x/832/2/167","title":"THE NANOGRAV NINE-YEAR DATA SET: MASS AND GEOMETRIC MEASUREMENTS OF BINARY MILLISECOND PULSARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":656,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Universities Space Research Association; National Science Foundation","keywords":"Pulsar; Physics; Millisecond pulsar; Neutron star; Binary pulsar; Astrophysics; Binary number; Orbital elements; Observatory; Gravitational wave; Astronomy","score_opus":0.044788347006594294,"score_gpt":0.32775456397781233,"score_spread":0.28296621697121804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2290284740","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9865936,0.00010300938,0.00044304904,0.000035285047,0.000013100106,0.000015610367,0.010805581,0.000045201767,0.0019455145],"genre_scores_gemma":[0.9579384,0.0000651878,0.0012680088,0.000029632778,0.000022615135,0.000036529258,0.039938007,0.000026747966,0.000674936],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995016,0.000056037225,0.00005064323,0.000119553944,0.00022338024,0.000048806574],"domain_scores_gemma":[0.99770564,0.0002666535,0.0008701308,0.00046078954,0.0004932899,0.000203424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00064957,0.00023261207,0.0002895816,0.002915851,0.0003760719,0.0005529288,0.0004594988,0.00027138868,0.00091540616],"category_scores_gemma":[0.0022202474,0.00015844891,0.00022644625,0.0021172715,0.00020740338,0.0005236559,0.00092784595,0.00024827317,0.0005578336],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015628111,0.000035858542,0.9853351,0.000024101808,0.000059182174,0.000065847424,0.000113000664,0.0008082794,0.0038802072,0.00013700362,0.0014016933,0.00798349],"study_design_scores_gemma":[0.0000091410975,0.000021763763,0.99585414,0.0000036301244,0.000012147856,0.000064228705,0.000048989117,0.0010750284,0.0006810065,0.000035300145,0.0021882749,0.0000063208727],"about_ca_topic_score_codex":0.010499633,"about_ca_topic_score_gemma":0.021361286,"teacher_disagreement_score":0.010499633,"about_ca_system_score_codex":0.00038666322,"about_ca_system_score_gemma":0.00020784466,"threshold_uncertainty_score":0.020877004},"labels":[],"label_agreement":null},{"id":"W2290991298","doi":"10.1088/0004-637x/813/2/81","title":"RADIALLY MAGNETIZED PROTOPLANETARY DISK: VERTICAL PROFILE","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Magnetic field; Magnetorotational instability; Accretion (finance); Magnetohydrodynamics; Instability; Planet; Ambipolar diffusion; Thin disk; Scale height","score_opus":0.014664309355391102,"score_gpt":0.23591161092907045,"score_spread":0.22124730157367936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2290991298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948671,0.000431514,0.0018369311,0.00004504954,0.000005960958,0.000008760905,0.00027602768,0.000059528942,0.0024691443],"genre_scores_gemma":[0.9983431,0.00014367298,0.0005192261,0.000012505335,0.000004140941,0.0000026772948,0.00014579139,0.000010856093,0.0008179302],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999776,0.0000020424238,7.894969e-7,0.000005383616,0.0000075773746,0.0000065341983],"domain_scores_gemma":[0.99993086,0.000011837062,0.00001995196,0.0000066458438,0.000021183365,0.000009519278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000037334063,0.00016126047,0.00011447116,0.00017730605,0.00011387671,0.00027249835,0.0001833318,0.00018500636,0.00076028943],"category_scores_gemma":[0.00017927361,0.00010278917,0.00010420558,0.00017473167,0.00010946223,0.00011757495,0.00015372677,0.00011508756,0.0001904867],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060165976,0.000098619974,0.050250433,0.00016553218,0.000064629945,0.000664124,0.00020157997,0.036634568,0.8837078,0.00091200956,0.000699065,0.025999995],"study_design_scores_gemma":[0.00009925873,0.0006195784,0.53975624,0.000045923764,0.000062872554,0.0013689687,0.00040914977,0.28912732,0.16163033,0.0011932759,0.005613797,0.00007316563],"about_ca_topic_score_codex":0.0021709206,"about_ca_topic_score_gemma":0.0016931093,"teacher_disagreement_score":0.0021709206,"about_ca_system_score_codex":0.00023987661,"about_ca_system_score_gemma":0.00007152056,"threshold_uncertainty_score":0.0043165684},"labels":[],"label_agreement":null},{"id":"W2291445857","doi":"10.3847/0004-637x/822/1/37","title":"ORDINARY X-RAYS FROM THREE EXTRAORDINARY MILLISECOND PULSARS: XMM-NEWTON OBSERVATIONS OF PSRs J0337+1715, J0636+5129, AND J0645+5158","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Millisecond pulsar; Pulsar; Physics; Astrophysics; White dwarf; Photometry (optics); Pulsar planet; Astronomy; Binary pulsar; Stars","score_opus":0.023834598040594953,"score_gpt":0.2910398805470876,"score_spread":0.26720528250649267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2291445857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999275,0.00006727875,0.000073119525,0.000009646472,0.0000022065615,0.0000030391163,0.00010750355,0.000006974216,0.00045517026],"genre_scores_gemma":[0.9989955,0.000044118005,0.00032919264,0.000016645474,0.00000820457,0.0000037360408,0.0004427731,0.000003875247,0.00015598856],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998549,0.000009808567,0.000014821613,0.000033797387,0.000053751406,0.000032948323],"domain_scores_gemma":[0.99968624,0.000025425139,0.00010050402,0.00003609315,0.00004697514,0.00010483496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002356855,0.00020759233,0.00029344612,0.00078811456,0.0005662479,0.0004779229,0.00023203726,0.00022269393,0.00071050005],"category_scores_gemma":[0.00031102623,0.00013543863,0.00017656271,0.00062603666,0.00028041034,0.0002697758,0.0006058262,0.00025970835,0.000200294],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033942296,0.000088410365,0.9054583,0.000035522622,0.00008781501,0.0006573416,0.0006999725,0.00024440655,0.08084537,0.00028375813,0.00036737457,0.010892347],"study_design_scores_gemma":[0.00001056974,0.000050686052,0.9967128,0.000002837272,0.000014930021,0.0002776049,0.00011869817,0.00016718288,0.0020070395,0.000046524554,0.0005877695,0.0000033342399],"about_ca_topic_score_codex":0.0034399522,"about_ca_topic_score_gemma":0.008362715,"teacher_disagreement_score":0.0034399522,"about_ca_system_score_codex":0.00033885584,"about_ca_system_score_gemma":0.00015474507,"threshold_uncertainty_score":0.0068398714},"labels":[],"label_agreement":null},{"id":"W2291746161","doi":"10.3847/0004-637x/821/2/86","title":"OF GENES AND MACHINES: APPLICATION OF A COMBINATION OF MACHINE LEARNING TOOLS TO ASTRONOMY DATA SETS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Galaxy; Redshift; Classifier (UML); Support vector machine; Photometric redshift; Data set; Set (abstract data type); Pattern recognition (psychology)","score_opus":0.012378280190914935,"score_gpt":0.23851270534762153,"score_spread":0.2261344251567066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2291746161","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04728484,0.0008238919,0.9398062,0.0015515343,0.0002295556,0.00021433369,0.00062529335,0.007342666,0.0021216276],"genre_scores_gemma":[0.19470058,0.00021514346,0.80226755,0.00039859547,0.00015233582,0.0002802947,0.00058381475,0.00044147775,0.00096026715],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99523646,0.0027460663,0.0002866588,0.0006922911,0.0009078255,0.00013070661],"domain_scores_gemma":[0.9855678,0.011505642,0.0005253446,0.0011854313,0.00092781516,0.00028806558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00636256,0.0012627617,0.0014445103,0.0041519064,0.0006982903,0.0022394399,0.0017033379,0.0012173685,0.0020643882],"category_scores_gemma":[0.021336753,0.0006490552,0.0016501915,0.0035353806,0.0014297686,0.0017033474,0.0021902972,0.0020517781,0.0007691578],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005435204,0.00047486532,0.027992437,0.00039544117,0.0007707604,0.0007956021,0.00086843007,0.22466263,0.0056655193,0.018815907,0.010774191,0.7082407],"study_design_scores_gemma":[0.000048270394,0.000063347085,0.0026901301,0.00002662632,0.000042417832,0.00010203437,0.000096943455,0.9649667,0.0014798616,0.027097318,0.0033635383,0.000022867585],"about_ca_topic_score_codex":0.0033882407,"about_ca_topic_score_gemma":0.0033296803,"teacher_disagreement_score":0.00636256,"about_ca_system_score_codex":0.0007596597,"about_ca_system_score_gemma":0.0009225823,"threshold_uncertainty_score":0.03364885},"labels":[],"label_agreement":null},{"id":"W2293492584","doi":"10.3847/0004-637x/831/2/184","title":"NEUTRON STAR MASS–RADIUS CONSTRAINTS OF THE QUIESCENT LOW-MASS X-RAY BINARIES X7 AND X5 IN THE GLOBULAR CLUSTER 47 TUC","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Neutron star; RADIUS; Astrophysics; Globular cluster; Low Mass; X-ray binary; Binary star; Stars","score_opus":0.00791824485637061,"score_gpt":0.20781513974682686,"score_spread":0.19989689489045626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2293492584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99929285,0.00006527138,0.00005926392,0.000008343667,8.184327e-7,0.000001130256,0.00005868278,0.000006967945,0.0005066476],"genre_scores_gemma":[0.9996742,0.000012264291,0.00006923165,0.0000045889888,0.0000020575908,0.0000013021368,0.00017934733,0.0000023782218,0.000054741166],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998658,0.000013133831,0.0000069387147,0.00003530107,0.000037314032,0.000041521267],"domain_scores_gemma":[0.9994574,0.00009068193,0.00015982159,0.000054944652,0.00007893918,0.000158231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027586424,0.00022944478,0.00038324832,0.0006941709,0.00063380675,0.0006993522,0.0004250327,0.00027167707,0.0013344358],"category_scores_gemma":[0.000575007,0.00012387641,0.00019554992,0.00032404144,0.00037239888,0.00019098846,0.00070476753,0.00015551544,0.00033592593],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055374583,0.00005785377,0.9322442,0.000042331565,0.00008625474,0.00033811363,0.00032247155,0.0017948023,0.058577307,0.0010773271,0.00036102755,0.0045444523],"study_design_scores_gemma":[0.000016957702,0.00007908662,0.98970836,0.000012466414,0.000027831733,0.00011326323,0.0002297518,0.0048624985,0.0041286326,0.00022186906,0.00059056655,0.000008685381],"about_ca_topic_score_codex":0.009024509,"about_ca_topic_score_gemma":0.012039449,"teacher_disagreement_score":0.009024509,"about_ca_system_score_codex":0.00071814435,"about_ca_system_score_gemma":0.00029008673,"threshold_uncertainty_score":0.017943919},"labels":[],"label_agreement":null},{"id":"W2295391252","doi":"10.3847/1538-4357/833/2/262","title":"CHEMICAL TAGGING CAN WORK: IDENTIFICATION OF STELLAR PHASE-SPACE STRUCTURES PURELY BY CHEMICAL-ABUNDANCE SIMILARITY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; South Carolina Department of Agriculture; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; European Commission; U.S. Department of Energy","keywords":"Stars; Abundance (ecology); Similarity (geometry); Space (punctuation); Identification (biology); Noise (video); Phase (matter)","score_opus":0.00981621971632838,"score_gpt":0.24732325684225254,"score_spread":0.23750703712592416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2295391252","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8948954,0.00033509146,0.0972879,0.00023027443,0.000046582307,0.000043532673,0.00042803868,0.00094366074,0.005789544],"genre_scores_gemma":[0.97602874,0.000049156675,0.022998568,0.00003898509,0.000016962806,0.000010139547,0.0003239666,0.0000635441,0.0004698512],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995034,0.0001436257,0.0000215816,0.00015278762,0.00011501337,0.000063683336],"domain_scores_gemma":[0.9976004,0.00055925484,0.00045482753,0.0006893746,0.00041358842,0.00028248533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012013018,0.00032811626,0.0005190137,0.0019778814,0.0006601627,0.0015406719,0.00039993817,0.00058023323,0.0018425084],"category_scores_gemma":[0.0055056857,0.00025488416,0.00026180365,0.0013403939,0.00093482225,0.001634086,0.0011172934,0.00031863502,0.0010714291],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023461292,0.00034376435,0.48786816,0.00025489237,0.00027791059,0.00018891496,0.0008996656,0.035425145,0.13090052,0.03162915,0.004677503,0.3051882],"study_design_scores_gemma":[0.00014037182,0.00047849581,0.34320495,0.000052983578,0.0001396472,0.00038904737,0.00066258,0.5220047,0.06730005,0.056150932,0.009320664,0.00015553356],"about_ca_topic_score_codex":0.0021887554,"about_ca_topic_score_gemma":0.0023786735,"teacher_disagreement_score":0.0021887554,"about_ca_system_score_codex":0.00039018242,"about_ca_system_score_gemma":0.000518932,"threshold_uncertainty_score":0.00635314},"labels":[],"label_agreement":null},{"id":"W2295413152","doi":"10.1088/0004-637x/767/1/48","title":"[O III] EMISSION AND GAS KINEMATICS IN A LYMAN-ALPHA BLOB AT<i>z</i>∼ 3.1","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Redshift; Galaxy; Emission spectrum; Offset (computer science); Line (geometry); Flux (metallurgy); Kinematics","score_opus":0.005757787803340258,"score_gpt":0.2057587260058817,"score_spread":0.20000093820254142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2295413152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994288,0.000054963144,0.00005012323,0.000008854121,4.701776e-7,0.0000010238291,0.000058850168,0.000011120202,0.00038565855],"genre_scores_gemma":[0.9993818,0.000044696088,0.00016022596,0.000013929059,0.0000024533688,0.0000015330303,0.00023066883,0.0000051058723,0.00015950786],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999505,0.0000026885964,0.0000014137363,0.000013999822,0.000008643971,0.00002259936],"domain_scores_gemma":[0.99976367,0.000014580993,0.000105812396,0.00000817366,0.00001997099,0.00008772549],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009320226,0.00021037033,0.00017400144,0.00079176953,0.00041937595,0.00052416424,0.00025710178,0.00020359326,0.0011616905],"category_scores_gemma":[0.00014438371,0.00017513365,0.000106182444,0.00047392794,0.00033131274,0.00025097255,0.0003997203,0.00025362385,0.00041471364],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040580772,0.000098820936,0.90207165,0.000021863882,0.000051010753,0.00038775103,0.00056741707,0.0004276601,0.09148205,0.0001412315,0.0003908082,0.0039539365],"study_design_scores_gemma":[0.0000039303723,0.000042988173,0.9984486,0.0000028334257,0.0000076154615,0.0001172327,0.000100111996,0.0004295588,0.00063559273,0.000023891545,0.00018489784,0.000002748438],"about_ca_topic_score_codex":0.011448224,"about_ca_topic_score_gemma":0.01400117,"teacher_disagreement_score":0.011448224,"about_ca_system_score_codex":0.00043567957,"about_ca_system_score_gemma":0.000085317864,"threshold_uncertainty_score":0.022763193},"labels":[],"label_agreement":null},{"id":"W2295535390","doi":"10.3847/0004-637x/826/2/124","title":"THE EVOLUTION OF THE INTRACLUSTER MEDIUM METALLICITY IN SUNYAEV ZEL’DOVICH-SELECTED GALAXY CLUSTERS AT 0 &lt; z &lt; 1.5","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Argonne National Laboratory; Strong; Space Telescope Science Institute; University of Chicago; Fermilab; Smithsonian Astrophysical Observatory; U.S. Department of Energy; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Metallicity; Intracluster medium; Galaxy cluster; Galaxy; Cluster (spacecraft); Galaxy formation and evolution; Galaxy groups and clusters","score_opus":0.004829467104530824,"score_gpt":0.19462007562725542,"score_spread":0.18979060852272459,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2295535390","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99941087,0.000045998917,0.000032566488,0.000015513688,0.0000013200112,0.000001555411,0.00020944563,0.000008934423,0.00027388593],"genre_scores_gemma":[0.99934894,0.000019769082,0.00003882088,0.0000073612864,0.000002451768,0.0000016431894,0.0004359264,0.0000053233753,0.0001397311],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987984,0.000008386673,0.000004808878,0.00003494634,0.000026328538,0.00004576054],"domain_scores_gemma":[0.9993961,0.000057575875,0.00022065786,0.00004130473,0.00006201876,0.00022235648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017816525,0.00017200923,0.00034307537,0.0014249838,0.0003365204,0.00073314056,0.00027975478,0.00017402253,0.001053896],"category_scores_gemma":[0.0004921711,0.00017437665,0.00019003695,0.0005386914,0.000336768,0.00019781022,0.0007582089,0.00017798273,0.00025930133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012062455,0.000014622021,0.98995376,0.000008958573,0.000047405494,0.00008597208,0.00023204208,0.00021517948,0.0067653987,0.00009326913,0.00026818007,0.0021946027],"study_design_scores_gemma":[0.0000023026737,0.0000065716667,0.99955004,8.968481e-7,0.0000035766623,0.000018156137,0.000044134835,0.00008913484,0.00015771278,0.000007900574,0.000118589385,0.0000010675788],"about_ca_topic_score_codex":0.010409915,"about_ca_topic_score_gemma":0.014194522,"teacher_disagreement_score":0.010409915,"about_ca_system_score_codex":0.0006283832,"about_ca_system_score_gemma":0.00016021718,"threshold_uncertainty_score":0.020698667},"labels":[],"label_agreement":null},{"id":"W2295569186","doi":"10.3847/0004-637x/821/2/113","title":"HIERARCHICAL FORMATION IN ACTION: CHARACTERIZING ACCELERATED GALAXY EVOLUTION IN COMPACT GROUPS USING WHOLE-SKY WISE DATA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"University of California, Los Angeles; National Aeronautics and Space Administration; California Institute of Technology; Office of Science; University of Utah; Jet Propulsion Laboratory; Alfred P. Sloan Foundation","keywords":"Galaxy; Physics; Sky; Astrophysics; Algorithm; Computer science","score_opus":0.045544860832444134,"score_gpt":0.2750052429561409,"score_spread":0.2294603821236968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2295569186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99596643,0.00003568677,0.00073012523,0.000019758336,0.0000013034982,0.000015033787,0.0023152425,0.0000576349,0.0008587494],"genre_scores_gemma":[0.99154,0.000017089103,0.0021014244,0.000015607971,0.0000061859164,0.000016924836,0.0058682035,0.000029321041,0.00040525754],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978894,0.000047476264,0.000013042806,0.00006240768,0.000039880128,0.000048253532],"domain_scores_gemma":[0.9984072,0.0002542441,0.00047109957,0.0002663343,0.00013422842,0.0004669358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005908092,0.00019276896,0.00017011538,0.0024399743,0.00023118351,0.0005667893,0.00031273536,0.00021442273,0.0015193983],"category_scores_gemma":[0.0015851484,0.00010218452,0.00031813054,0.0013031561,0.00021674276,0.00049174577,0.0009119426,0.00022424161,0.0006130572],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011630241,0.00005202988,0.9869594,0.000014147983,0.000052573156,0.000056468263,0.00028140369,0.0009806472,0.003980586,0.00025454193,0.00072097144,0.006530916],"study_design_scores_gemma":[0.00000244268,0.00003011483,0.9962991,0.0000019731685,0.000007870027,0.000043010565,0.00014858974,0.0023789587,0.0004911605,0.00010677601,0.00048676325,0.0000033236513],"about_ca_topic_score_codex":0.0066155214,"about_ca_topic_score_gemma":0.0082644895,"teacher_disagreement_score":0.0066155214,"about_ca_system_score_codex":0.0002259321,"about_ca_system_score_gemma":0.00014038103,"threshold_uncertainty_score":0.01315403},"labels":[],"label_agreement":null},{"id":"W2295717594","doi":"10.3847/0004-637x/822/1/13","title":"RADIO SYNCHROTRON FLUCTUATION STATISTICS AS A PROBE OF MAGNETIZED INTERSTELLAR TURBULENCE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Synchrotron; Turbulence; Mach number; Astrophysics; Synchrotron radiation; Magnetic field; Polarization (electrochemistry); Interstellar medium; Computational physics; Galaxy; Optics; Mechanics","score_opus":0.007125434531740811,"score_gpt":0.2294715047035004,"score_spread":0.22234607017175959,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2295717594","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99795854,0.000017415137,0.0015588558,0.000014530478,0.0000020003476,0.0000016360499,0.0000743375,0.00003903952,0.0003337516],"genre_scores_gemma":[0.9997055,0.0000035564144,0.00021690226,0.0000016363681,0.000001481477,6.2400557e-7,0.00003939952,0.0000035008768,0.000027374897],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998963,0.00003425862,0.000005581005,0.00002775462,0.000022173204,0.0000139694685],"domain_scores_gemma":[0.99895513,0.0003682782,0.0003222597,0.00011655088,0.00011639915,0.000121487436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039951803,0.00020820207,0.00023391693,0.000433541,0.00011145024,0.0005186395,0.00017410518,0.00014600242,0.00034934297],"category_scores_gemma":[0.0020760016,0.0001448726,0.00012981353,0.00032497945,0.00028165895,0.0004084409,0.00023669348,0.0002384694,0.00006846608],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083701755,0.00016713838,0.6774244,0.000035664805,0.00021648609,0.00029176165,0.00020698621,0.11687076,0.18560086,0.006214634,0.00039293297,0.011741344],"study_design_scores_gemma":[0.00003436584,0.00026682223,0.7368467,0.000006279876,0.000029674859,0.00011423969,0.000084605,0.24460384,0.0159009,0.0017663719,0.00029801787,0.000048258913],"about_ca_topic_score_codex":0.0006509741,"about_ca_topic_score_gemma":0.0005384932,"teacher_disagreement_score":0.0006509741,"about_ca_system_score_codex":0.00021242404,"about_ca_system_score_gemma":0.00008875948,"threshold_uncertainty_score":0.0021128654},"labels":[],"label_agreement":null},{"id":"W2296403033","doi":"10.3847/0004-637x/822/1/51","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY XVI: THE ANGULAR MOMENTUM OF DWARF EARLY-TYPE GALAXIES FROM GLOBULAR CLUSTER SATELLITES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Virgo Cluster; Velocity dispersion; Dwarf galaxy; Galaxy; Cluster (spacecraft); Star cluster; Amplitude; Angular momentum","score_opus":0.01942153409934096,"score_gpt":0.22074540803613252,"score_spread":0.20132387393679155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2296403033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99683577,0.00017169751,0.0005423757,0.000043549975,0.0000039127112,0.00000743968,0.0016255794,0.000040481198,0.00072917115],"genre_scores_gemma":[0.99630874,0.000045148947,0.0007613199,0.000011244509,0.0000043240743,0.0000055517553,0.002680209,0.000011185075,0.00017217771],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998374,0.00003476413,0.000006700728,0.00003743448,0.00004723815,0.000036466627],"domain_scores_gemma":[0.9994803,0.00012518691,0.000105968196,0.000091747184,0.0000824294,0.000114363545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006682593,0.00024764834,0.00024065273,0.0014226713,0.00023468182,0.00047360797,0.00038235408,0.00027583633,0.0006667583],"category_scores_gemma":[0.0011249337,0.0001373625,0.0004191975,0.0009987758,0.00016950592,0.00029802523,0.00046624924,0.00016716987,0.00025609726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079358084,0.000021285834,0.98019034,0.00001679776,0.00011165304,0.00006286668,0.000045041703,0.013081079,0.001669381,0.0001943414,0.0004898824,0.0040381574],"study_design_scores_gemma":[0.0000055160594,0.00001628846,0.98248315,0.0000066871557,0.000025238263,0.000028133096,0.00004408946,0.016152283,0.0005273638,0.000107060834,0.00059663877,0.000007639185],"about_ca_topic_score_codex":0.020155294,"about_ca_topic_score_gemma":0.02512861,"teacher_disagreement_score":0.020155294,"about_ca_system_score_codex":0.00061041984,"about_ca_system_score_gemma":0.0002493799,"threshold_uncertainty_score":0.040075958},"labels":[],"label_agreement":null},{"id":"W2296465908","doi":"10.3847/0004-637x/831/1/13","title":"URCA COOLING PAIRS IN THE NEUTRON STAR OCEAN AND THEIR EFFECT ON SUPERBURSTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Neutron star; Physics; Neutrino; Astrophysics; Thermonuclear fusion; Luminosity; Accretion (finance); Nuclear physics; Plasma; Galaxy","score_opus":0.007925970940636205,"score_gpt":0.2137064499451579,"score_spread":0.20578047900452168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2296465908","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994467,0.00008700808,0.00007898487,0.000014816254,0.0000027781737,0.000001093627,0.000033806242,0.00000554131,0.00032935044],"genre_scores_gemma":[0.99975115,0.000031883155,0.000053511078,0.000008490616,0.0000016248852,0.0000012236629,0.00004569569,0.00000384378,0.000102647195],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998841,0.000019960522,0.000006893897,0.00003102244,0.00002264448,0.000035315996],"domain_scores_gemma":[0.9991604,0.00019086436,0.00032669815,0.000077495635,0.000078881334,0.00016568972],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023733095,0.00022908782,0.00037515897,0.00035998074,0.00033592834,0.0005567505,0.00022959315,0.0002653588,0.0013576929],"category_scores_gemma":[0.0011300332,0.00019035341,0.0002111706,0.00021218415,0.0003673503,0.00033448866,0.0006950761,0.0004022114,0.00015772476],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001726883,0.000098610224,0.7932795,0.000043688804,0.0000928953,0.0005171134,0.00034202327,0.0012976961,0.19308811,0.00034169658,0.00013728696,0.009034436],"study_design_scores_gemma":[0.0000126304885,0.00012673135,0.984567,0.000005615698,0.000019596278,0.00024328414,0.0002552822,0.0013740391,0.012848529,0.00017451955,0.0003662347,0.000006618707],"about_ca_topic_score_codex":0.002251617,"about_ca_topic_score_gemma":0.0025087066,"teacher_disagreement_score":0.002251617,"about_ca_system_score_codex":0.00026514358,"about_ca_system_score_gemma":0.00013657937,"threshold_uncertainty_score":0.004541993},"labels":[],"label_agreement":null},{"id":"W2299876970","doi":"10.3847/0004-637x/824/1/18","title":"SPINNING DUST EMISSION FROM ULTRA-SMALL SILICATES: EMISSIVITY AND POLARIZATION SPECTRUM","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Emissivity; Polarization (electrochemistry); Rotational temperature; Spinning; Silicate; Cosmic dust; Cosmic microwave background; Population","score_opus":0.010655664049079423,"score_gpt":0.22303430659836856,"score_spread":0.21237864254928915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2299876970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953467,0.000118888696,0.0035888888,0.000013784644,0.00000294505,0.0000024674255,0.000069156435,0.000020388397,0.00083677133],"genre_scores_gemma":[0.9996872,0.000019817857,0.00022491005,0.0000018249483,0.0000015932366,6.888067e-7,0.000027009199,0.0000013418355,0.000035684156],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999442,0.000008107123,0.0000022882027,0.00002324242,0.00001207039,0.000010092596],"domain_scores_gemma":[0.9998627,0.000043091073,0.00004489647,0.000017297365,0.00001904424,0.000012971595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011010237,0.0001956081,0.00008187997,0.00042042971,0.00009522058,0.00021268589,0.00014341882,0.00016431231,0.00053238455],"category_scores_gemma":[0.00023515712,0.000092801674,0.00014377182,0.00017240577,0.0003186092,0.00024211901,0.00015288347,0.00009464854,0.00007563763],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000268965,0.00004658989,0.26254866,0.00005520385,0.00006844399,0.000302815,0.00009050456,0.00814484,0.7182192,0.0022331018,0.00017910011,0.00784266],"study_design_scores_gemma":[0.00002563624,0.00014022613,0.5566678,0.000012913425,0.000057787976,0.001017387,0.00025810456,0.118836045,0.31776452,0.0037871008,0.0013977038,0.000034774268],"about_ca_topic_score_codex":0.00029214416,"about_ca_topic_score_gemma":0.0001677119,"teacher_disagreement_score":0.00053238455,"about_ca_system_score_codex":0.000091122565,"about_ca_system_score_gemma":0.000025415236,"threshold_uncertainty_score":0.0017810464},"labels":[],"label_agreement":null},{"id":"W2300756355","doi":"10.3847/0004-637x/822/2/80","title":"THE REDSHIFT DISTRIBUTION OF DUSTY STAR-FORMING GALAXIES FROM THE SPT SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":152,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"","keywords":"Physics; Redshift; Astrophysics; Galaxy; Astronomy; Redshift survey; Gravitational lens; Submillimeter Array; South Pole Telescope; Star formation","score_opus":0.010619246888643775,"score_gpt":0.2139645923399609,"score_spread":0.20334534545131713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2300756355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981293,0.00005470256,0.000113182694,0.000025292939,0.0000015964195,0.0000042841043,0.0010198803,0.000019293064,0.00063253974],"genre_scores_gemma":[0.9970476,0.000057273748,0.00017133387,0.000012094611,0.0000074858754,0.0000067899964,0.0024830808,0.0000070385818,0.00020726142],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967134,0.00004218608,0.00002495065,0.00009559273,0.00011832981,0.00004763607],"domain_scores_gemma":[0.99842453,0.00020759694,0.00058664207,0.000167451,0.0003004736,0.0003133096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003232845,0.00016510196,0.00020401552,0.0025921157,0.0002431554,0.0005774139,0.0002934702,0.00019728544,0.0018787126],"category_scores_gemma":[0.0015118956,0.00012336728,0.00019962192,0.0016295173,0.00028615617,0.00033941324,0.0006171498,0.00023132133,0.00040416562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022194998,0.000008734695,0.9941514,0.0000057512116,0.000020621275,0.00005109391,0.00016632062,0.000084307285,0.0015700031,0.000049316055,0.00030102674,0.0035692302],"study_design_scores_gemma":[0.000001042793,0.000007582116,0.99955326,9.21964e-7,0.0000023450875,0.000051886305,0.000036472644,0.000104664185,0.00009434355,0.000009861143,0.00013683864,8.073194e-7],"about_ca_topic_score_codex":0.00539304,"about_ca_topic_score_gemma":0.005762093,"teacher_disagreement_score":0.00539304,"about_ca_system_score_codex":0.00026982056,"about_ca_system_score_gemma":0.00011617762,"threshold_uncertainty_score":0.010723293},"labels":[],"label_agreement":null},{"id":"W2301650955","doi":"10.3847/0004-637x/822/2/96","title":"PSR B0329+54: STATISTICS OF SUBSTRUCTURE DISCOVERED WITHIN THE SCATTERING DISK ON RADIOASTRON BASELINES OF UP TO 235,000 km","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Scattering; Substructure; Visibility; Envelope (radar); Interferometry; Correlation function (quantum field theory); Range (aeronautics); Radio wave","score_opus":0.008553845372764513,"score_gpt":0.22950610947741304,"score_spread":0.22095226410464852,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2301650955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99844754,0.000072481926,0.0001582005,0.000020639465,0.000002240005,0.000002229243,0.00078886765,0.00003995315,0.0004677295],"genre_scores_gemma":[0.9985145,0.000018532166,0.0001005489,0.0000038668295,0.00000521661,0.0000023615396,0.0012896301,0.000008352719,0.000057036614],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976176,0.00002357812,0.000019217969,0.00008329678,0.00006555684,0.000046685618],"domain_scores_gemma":[0.9989102,0.00017064736,0.00041305978,0.00013583062,0.00013241764,0.00023784972],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034195112,0.00017640185,0.0003514339,0.001326362,0.00026979664,0.00049333216,0.0002516612,0.00024626454,0.0010720667],"category_scores_gemma":[0.0011863303,0.00016688509,0.0002342305,0.00096847,0.00021569672,0.0002716061,0.00048911734,0.0001933416,0.00029887198],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030145788,0.000031588133,0.9614972,0.00002884843,0.000115650306,0.00026662645,0.00017016137,0.002084801,0.027733188,0.00022483974,0.00079093827,0.0067546614],"study_design_scores_gemma":[0.0000035923779,0.000013686832,0.99794537,0.0000016660701,0.000009047358,0.00006779761,0.000031194682,0.0011646379,0.00048905547,0.000028594279,0.00024109003,0.0000043130744],"about_ca_topic_score_codex":0.0059687477,"about_ca_topic_score_gemma":0.0061045852,"teacher_disagreement_score":0.0059687477,"about_ca_system_score_codex":0.000344713,"about_ca_system_score_gemma":0.00011399122,"threshold_uncertainty_score":0.011868},"labels":[],"label_agreement":null},{"id":"W2302048883","doi":"10.3847/0004-637x/820/2/100","title":"RADIO POLARIZATION OBSERVATIONS OF THE SNAIL: A CRUSHED PULSAR WIND NEBULA IN G327.1–1.1 WITH A HIGHLY ORDERED MAGNETIC FIELD","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Pulsar wind nebula; Pulsar; Ejecta; Magnetic field; Supernova; Polarization (electrochemistry); Nebula; Supernova remnant; Heliosphere","score_opus":0.010502760372567605,"score_gpt":0.25896532503505404,"score_spread":0.24846256466248642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2302048883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99975294,0.000011970113,0.000096683354,0.000004457506,7.703867e-7,0.0000012690257,0.000019977786,0.0000046484906,0.00010738227],"genre_scores_gemma":[0.9996964,0.000009402904,0.00016219074,0.0000045110246,0.0000012244808,0.0000015479595,0.00006945215,0.000002151446,0.000053172713],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.0000050725394,0.0000013742925,0.000009558941,0.000008135043,0.0000077208],"domain_scores_gemma":[0.9998691,0.000021321495,0.000037264905,0.000014765391,0.00001647624,0.00004104213],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011706649,0.00014653464,0.00016781349,0.00031163354,0.0001852065,0.00022972279,0.00019486996,0.0001984809,0.00040143167],"category_scores_gemma":[0.00017008765,0.00014742235,0.00012422571,0.00018701404,0.00030374533,0.000100222525,0.0003272085,0.00020303905,0.000089448484],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030178958,0.00015224247,0.4306882,0.000037244772,0.00008632797,0.0023889292,0.0003328335,0.0028318989,0.5569577,0.00033628155,0.00026624431,0.0056203622],"study_design_scores_gemma":[0.000024407344,0.0001609937,0.9829428,0.0000043017467,0.000022759366,0.0010098658,0.00016471492,0.006568443,0.008562695,0.00011635444,0.00041446308,0.000008141271],"about_ca_topic_score_codex":0.0012531005,"about_ca_topic_score_gemma":0.0018978918,"teacher_disagreement_score":0.0012531005,"about_ca_system_score_codex":0.00013681778,"about_ca_system_score_gemma":0.000060009635,"threshold_uncertainty_score":0.002491653},"labels":[],"label_agreement":null},{"id":"W2303591519","doi":"10.3847/0004-637x/825/1/66","title":"BICEP2/KECK ARRAY. VII. MATRIX BASED E/B SEPARATION APPLIED TO BICEP2 AND THE KECK ARRAY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; University of British Columbia; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Astronomy; Optics; Astrophysics","score_opus":0.006718119128736309,"score_gpt":0.2387347489860828,"score_spread":0.23201662985734647,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2303591519","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3114975,0.00041507903,0.64337194,0.00061675784,0.00022738209,0.00013302767,0.003793245,0.00621063,0.03373457],"genre_scores_gemma":[0.507544,0.00015634616,0.47992763,0.00017774505,0.000057964156,0.00014887897,0.0033686333,0.0007037721,0.007915141],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997391,0.00005753635,0.000011769916,0.00004539345,0.000097492455,0.000048630725],"domain_scores_gemma":[0.9996456,0.000071463925,0.000039799263,0.00009814161,0.000113286005,0.000031609627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055439566,0.00059258397,0.0002527946,0.0008215166,0.00047345835,0.0009274119,0.0004980353,0.00050363695,0.0046192044],"category_scores_gemma":[0.001587748,0.0002915415,0.00035143408,0.0012950536,0.0003074281,0.00086915825,0.001020358,0.0006559914,0.0015177418],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002313424,0.00019936466,0.0185364,0.0004939118,0.00031714814,0.001114715,0.0005255919,0.11474917,0.26283926,0.050716527,0.017639672,0.5305548],"study_design_scores_gemma":[0.0001273684,0.00017495912,0.055162575,0.000044866163,0.0000782747,0.0010633998,0.0002754455,0.66508985,0.21180472,0.023634974,0.04236801,0.00017566065],"about_ca_topic_score_codex":0.003373584,"about_ca_topic_score_gemma":0.0055421297,"teacher_disagreement_score":0.0046192044,"about_ca_system_score_codex":0.00027145597,"about_ca_system_score_gemma":0.0004619382,"threshold_uncertainty_score":0.015452802},"labels":[],"label_agreement":null},{"id":"W2304639917","doi":"10.3847/0004-637x/822/2/82","title":"HIGHLY EXCITED H<sub>2</sub> IN HERBIG–HARO 7: FORMATION PUMPING IN SHOCKED MOLECULAR GAS?","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Herbig–Haro object; Physics; Excited state; Atomic physics; Dissociation (chemistry); Astrophysics; Excitation; Shock wave; Emission spectrum; Spectral line; Excitation temperature; Spectrograph; Bow shock (aerodynamics); Chemistry; Astronomy","score_opus":0.008113486077757227,"score_gpt":0.2182099937732908,"score_spread":0.2100965076955336,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2304639917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99928683,0.00005809774,0.0002845237,0.000028454635,0.0000025040567,0.0000023369041,0.000031984597,0.000016858348,0.00028842772],"genre_scores_gemma":[0.9995778,0.000020309122,0.00013344381,0.000028194945,0.0000023312912,0.0000017197306,0.000085145984,0.000004999561,0.00014609605],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999249,0.000004272299,0.0000020988473,0.000015580934,0.000010659701,0.00004246313],"domain_scores_gemma":[0.99987817,0.000023448869,0.000032228396,0.0000129791215,0.000020386375,0.0000327835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001813242,0.00019909769,0.0002794261,0.0002749468,0.00041996283,0.00060017477,0.00049831095,0.00042259126,0.0019575758],"category_scores_gemma":[0.00021860756,0.0002044221,0.00016496239,0.00025533268,0.0003258183,0.00033179225,0.00039860752,0.0004223442,0.00022968929],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000548652,0.000167564,0.21409911,0.00006151878,0.00013426179,0.0014790539,0.00026057687,0.0026760173,0.77196014,0.0008474987,0.00040538347,0.007360245],"study_design_scores_gemma":[0.000060306742,0.00023058332,0.85092074,0.000019739104,0.00006857438,0.00030247724,0.00054129184,0.018631095,0.12723136,0.0006503005,0.0013137779,0.000029749299],"about_ca_topic_score_codex":0.002084704,"about_ca_topic_score_gemma":0.0024365808,"teacher_disagreement_score":0.002084704,"about_ca_system_score_codex":0.00034824418,"about_ca_system_score_gemma":0.00008843303,"threshold_uncertainty_score":0.0065487027},"labels":[],"label_agreement":null},{"id":"W2304899920","doi":"10.3847/0004-637x/823/1/28","title":"SIMULATING THE FORMATION OF MASSIVE PROTOSTARS. I. RADIATIVE FEEDBACK AND ACCRETION DISKS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Protostar; Radiative transfer; Accretion (finance); Outflow; Stars; Star formation; Accretion disc; Gravitation; Gravitational collapse","score_opus":0.012255327506373542,"score_gpt":0.2483334378075247,"score_spread":0.23607811030115117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2304899920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938048,0.00005071096,0.0017443679,0.000101828635,0.000016855432,0.000027780558,0.00014209132,0.00010044152,0.0040111295],"genre_scores_gemma":[0.9968958,0.000032282525,0.001970391,0.000051927218,0.0000064419346,0.000024731931,0.00014879335,0.000024967183,0.0008447083],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989986,0.00002450336,0.0000041474736,0.0000141904675,0.000018939461,0.00003830064],"domain_scores_gemma":[0.99954456,0.00018874223,0.00007298331,0.000030947198,0.000052677507,0.00010997148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023805798,0.00035855832,0.00040706815,0.00027605525,0.00049210846,0.00059098634,0.0010769597,0.00089407543,0.0015717436],"category_scores_gemma":[0.0011948085,0.000297161,0.00046883684,0.00029302342,0.0007640466,0.00041558925,0.0006032772,0.0005904718,0.00015849924],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022749302,0.00019098441,0.0133812735,0.000030618852,0.00005150168,0.00025058072,0.00012903946,0.9761027,0.004889306,0.002285625,0.00035725324,0.0021036856],"study_design_scores_gemma":[0.00012048013,0.00010777124,0.0027340227,0.0000049806304,0.000011169673,0.000032555192,0.000070449976,0.9948684,0.0011226535,0.0005208823,0.00039619365,0.000010381169],"about_ca_topic_score_codex":0.016455004,"about_ca_topic_score_gemma":0.008456644,"teacher_disagreement_score":0.016455004,"about_ca_system_score_codex":0.0009898522,"about_ca_system_score_gemma":0.0007358498,"threshold_uncertainty_score":0.03271842},"labels":[],"label_agreement":null},{"id":"W2306903250","doi":"10.3847/0004-637x/824/1/57","title":"IN-N-OUT: THE GAS CYCLE FROM DWARFS TO SPIRAL GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":193,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Halo; Galaxy; Galactic halo; Accretion (finance); Spiral galaxy; Stellar mass; Galaxy formation and evolution; Baryon; Elliptical galaxy","score_opus":0.007666077236759272,"score_gpt":0.21619158475517317,"score_spread":0.2085255075184139,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2306903250","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973296,0.000089579684,0.0008220109,0.000115103016,0.000008876841,0.0000043743016,0.00019176822,0.000056893896,0.0013818009],"genre_scores_gemma":[0.99907315,0.00003453685,0.00034745855,0.000036981182,0.000004084488,0.000003400061,0.00022898469,0.000022005948,0.00024934282],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998983,0.000035315858,0.000005107055,0.000024850393,0.00001293522,0.000023427636],"domain_scores_gemma":[0.99946886,0.0001665936,0.00008806848,0.00009005127,0.000063112515,0.0001233399],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000565774,0.00034139154,0.00038895907,0.00031328117,0.0004533205,0.00074048765,0.0006271155,0.00032269268,0.0014550851],"category_scores_gemma":[0.002728655,0.00015694195,0.00044497213,0.00028464574,0.00061301276,0.000647601,0.00051213097,0.00037292804,0.00011311696],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042980863,0.00018826043,0.23307315,0.00011921407,0.00034723876,0.00038722917,0.0004338693,0.7253202,0.014067869,0.013095136,0.0023932655,0.01014479],"study_design_scores_gemma":[0.00022267617,0.00026475775,0.09841399,0.000037704,0.00011683658,0.00018113841,0.00041026156,0.8807036,0.005097118,0.01115489,0.0033510737,0.000045968172],"about_ca_topic_score_codex":0.017068565,"about_ca_topic_score_gemma":0.016223475,"teacher_disagreement_score":0.017068565,"about_ca_system_score_codex":0.00083911006,"about_ca_system_score_gemma":0.00047507614,"threshold_uncertainty_score":0.033938408},"labels":[],"label_agreement":null},{"id":"W2308996868","doi":"10.3847/0004-637x/832/1/95","title":"COSMOLOGICAL CONSTRAINTS FROM GALAXY CLUSTERS IN THE 2500 SQUARE-DEGREE SPT-SZ SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":264,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Université de Montréal; Canadian Institute for Advanced Research; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; Smithsonian Astrophysical Observatory; Bundesministerium für Wirtschaft und Technologie; Canada Research Chairs; Danmarks Grundforskningsfond; National Science Foundation; Compute Canada; University of Chicago; McGill University; Argonne National Laboratory; U.S. Department of Energy; Gordon and Betty Moore Foundation; Deutsche Forschungsgemeinschaft; National Research Foundation; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; Smithsonian Institution","keywords":"Physics; Planck; South Pole Telescope; Cosmic microwave background; Astrophysics; CMB cold spot; Dark energy; Galaxy cluster; Cosmology; Sunyaev–Zel'dovich effect; Redshift; Omega; Neutrino; Hubble's law; Galaxy; Sigma; Astronomy; Particle physics; Anisotropy; Quantum mechanics","score_opus":0.027620719080842526,"score_gpt":0.2638464659111921,"score_spread":0.23622574683034958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2308996868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973418,0.000049047332,0.00056424446,0.000035198398,0.0000022106992,0.0000022889042,0.0008352777,0.000012024679,0.0011578422],"genre_scores_gemma":[0.9981146,0.000023172654,0.0002483301,0.0000074741583,0.0000031248285,0.0000017367477,0.0015121972,0.0000041337444,0.00008535826],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995184,0.00011320496,0.000024513174,0.0001134252,0.00013718326,0.00009330324],"domain_scores_gemma":[0.99809045,0.0006229028,0.0004818934,0.00026679804,0.00019952716,0.00033845945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007524578,0.00027009752,0.00034891,0.0012078707,0.00050190237,0.0008798547,0.00031286062,0.00016232741,0.0022736294],"category_scores_gemma":[0.0033580463,0.00019215164,0.00032088815,0.0014872454,0.00041219394,0.0002752736,0.0008629527,0.00021911193,0.00021699876],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002684506,0.000020527665,0.97166955,0.000032956228,0.00016454293,0.00014553081,0.00015864767,0.013596177,0.004755005,0.0024312225,0.0011203664,0.0056370497],"study_design_scores_gemma":[0.000018179266,0.000021943632,0.9858758,0.000011371467,0.000036429457,0.0000651037,0.00013637169,0.010309073,0.0014219359,0.0005760636,0.0015147729,0.000013003081],"about_ca_topic_score_codex":0.02308031,"about_ca_topic_score_gemma":0.030765096,"teacher_disagreement_score":0.02308031,"about_ca_system_score_codex":0.00043356247,"about_ca_system_score_gemma":0.00053771725,"threshold_uncertainty_score":0.04589194},"labels":[],"label_agreement":null},{"id":"W2313334018","doi":"10.3847/0004-637x/829/2/133","title":"FARADAY ROTATION MEASURE SYNTHESIS OF INTERMEDIATE REDSHIFT QUASARS AS A PROBE OF INTERVENING MATTER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Faraday effect; Quasar; Redshift; Polarization (electrochemistry); Faraday cage; Line-of-sight; Polarimetry; Spectral line; Sky","score_opus":0.007805497213891589,"score_gpt":0.21466369271925495,"score_spread":0.20685819550536336,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2313334018","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976494,0.000064443426,0.0011168395,0.000008823711,0.0000013288453,0.0000035910728,0.00026032372,0.000019776364,0.00087543105],"genre_scores_gemma":[0.99931395,0.000014855286,0.00036117423,0.0000026650625,0.0000025669137,0.0000019308106,0.00022532708,0.0000032201838,0.00007432575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998149,0.000040555507,0.00001603756,0.00005093198,0.00004574073,0.000031697546],"domain_scores_gemma":[0.99827516,0.00035104476,0.0007876408,0.00020156633,0.00018151084,0.00020304108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036897248,0.00021644992,0.00022304006,0.0016153405,0.00019907964,0.00063528813,0.00013660216,0.00013266581,0.0013461334],"category_scores_gemma":[0.0015869803,0.00009032017,0.00014905464,0.00074421655,0.00030543742,0.00026306196,0.00047532498,0.00018415225,0.00020076188],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020424025,0.000039175513,0.8939752,0.000042303684,0.000104546474,0.000112481954,0.00032481094,0.0006755698,0.08560521,0.0006481958,0.00013225382,0.018136026],"study_design_scores_gemma":[0.0000013522852,0.00002818169,0.99744284,0.0000011052871,0.0000060441985,0.00003964905,0.000050384773,0.0002942397,0.0018868165,0.000087068125,0.0001591943,0.0000029863081],"about_ca_topic_score_codex":0.0009726871,"about_ca_topic_score_gemma":0.0014346248,"teacher_disagreement_score":0.0016153405,"about_ca_system_score_codex":0.00017456149,"about_ca_system_score_gemma":0.000058919715,"threshold_uncertainty_score":0.0045033097},"labels":[],"label_agreement":null},{"id":"W2315247424","doi":"10.1088/0004-637x/733/1/73","title":"ERRATUM: “GRAVITATIONAL LENS MODELING WITH GENETIC ALGORITHMS AND PARTICLE SWARM OPTIMIZERS” (2011, ApJ, 727, 80)","year":2011,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Optical Polarization and Ellipsometry","field":"Engineering","cited_by":1,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Particle swarm optimization; Gravitation; Genetic algorithm; Statistical physics; Algorithm; Astrophysics; Astronomy; Machine learning; Computer science","score_opus":0.016126892078655117,"score_gpt":0.2090130137453702,"score_spread":0.1928861216667151,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2315247424","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00054736243,0.0017827069,0.002527011,0.04780103,0.93255156,0.000042023763,0.0019427348,0.00068258453,0.012123014],"genre_scores_gemma":[0.028380884,0.008239603,0.017508686,0.08408904,0.2576374,0.00024117189,0.0090168305,0.0034151995,0.59147114],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9981647,0.0002652457,0.00032482937,0.00027932425,0.00084826746,0.000117592106],"domain_scores_gemma":[0.99339586,0.0013862514,0.00042926378,0.0006010305,0.0038532922,0.0003342172],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016523808,0.0024556315,0.0017073929,0.002994709,0.0037203105,0.0038657738,0.0030652375,0.0054824897,0.05444354],"category_scores_gemma":[0.02511898,0.0008975647,0.0016030166,0.0024142093,0.0017582747,0.003805096,0.0020550124,0.0060572666,0.02722132],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004194618,0.0000069403504,0.00007170197,0.00005942834,0.000011354066,0.0001577891,0.000012358372,0.00018350103,0.00007668685,0.001884151,0.9925211,0.004973011],"study_design_scores_gemma":[0.00007846196,0.000061725674,0.0015378282,0.00026508785,0.00006310004,0.0007084558,0.00013536419,0.002732314,0.0011083636,0.009608632,0.98360544,0.00009533938],"about_ca_topic_score_codex":0.01799709,"about_ca_topic_score_gemma":0.02367693,"teacher_disagreement_score":0.05444354,"about_ca_system_score_codex":0.003284066,"about_ca_system_score_gemma":0.00278932,"threshold_uncertainty_score":0.18213177},"labels":[],"label_agreement":null},{"id":"W2316036685","doi":"10.1088/0004-637x/777/1/80","title":"ERRATUM: “STUDIES OF VARIABILITY IN PROTO-PLANETARY NEBULAE. II. LIGHT AND VELOCITY CURVE ANALYSES OF IRAS 22272+5435 AND 22223+4327” (2013, ApJ, 766, 116)","year":2013,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Planetary nebula; Astrophysics; Astronomy; Stars","score_opus":0.025849792581234904,"score_gpt":0.27631452571407855,"score_spread":0.2504647331328437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2316036685","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0009842807,0.001406514,0.00053341786,0.04076272,0.92829937,0.000054614637,0.0058956426,0.00066922116,0.021394257],"genre_scores_gemma":[0.014050937,0.007118359,0.0045983256,0.05224219,0.13795397,0.00018099231,0.018588804,0.002786606,0.76247984],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99772733,0.00018117506,0.0004703579,0.00024229988,0.0012346645,0.00014407857],"domain_scores_gemma":[0.9812471,0.0022387977,0.0008302094,0.0011017531,0.013918846,0.00066334713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018481427,0.0014217334,0.0012132637,0.00345932,0.0040787635,0.0028428435,0.0019137884,0.0026420448,0.062050395],"category_scores_gemma":[0.024136974,0.0007239053,0.001051684,0.0026513985,0.0010296877,0.0021069169,0.0017568986,0.003966968,0.04471343],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002012829,0.0000069380167,0.00013191902,0.00005522322,0.0000037110156,0.000102562626,0.000014763011,0.000023314378,0.000059978487,0.00019943756,0.99583614,0.0035459436],"study_design_scores_gemma":[0.000018188104,0.000019611696,0.003123369,0.00020260336,0.000021700986,0.00020167226,0.000107317544,0.00009345319,0.00044352794,0.00041993466,0.9953177,0.000031092313],"about_ca_topic_score_codex":0.041972812,"about_ca_topic_score_gemma":0.06304548,"teacher_disagreement_score":0.062050395,"about_ca_system_score_codex":0.0028352044,"about_ca_system_score_gemma":0.0045124884,"threshold_uncertainty_score":0.20757926},"labels":[],"label_agreement":null},{"id":"W2317893021","doi":"10.1088/0004-637x/701/2/2035","title":"ERRATUM: “<i>SUZAKU</i>OBSERVATIONS OF LOCAL ULTRALUMINOUS INFRARED GALAXIES” (2009, ApJ, 691, 261)","year":2009,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Astrophysics; Galaxy; Physics; Luminous infrared galaxy","score_opus":0.01488271821498286,"score_gpt":0.2276032492124883,"score_spread":0.21272053099750546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2317893021","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00965346,0.0054292665,0.0033679092,0.05816569,0.8665914,0.00015261746,0.028859396,0.0026148658,0.025165427],"genre_scores_gemma":[0.07872726,0.015556902,0.02987077,0.1230129,0.1399708,0.00062699185,0.12683189,0.0060674376,0.4793351],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9989524,0.00009372445,0.00022134777,0.00019058073,0.0004215789,0.00012036272],"domain_scores_gemma":[0.9925115,0.00090256095,0.0010080686,0.0008242471,0.0043123704,0.00044119652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001093595,0.0015443923,0.0007853871,0.0036499451,0.0027274028,0.0020978586,0.001964914,0.0019190283,0.040318087],"category_scores_gemma":[0.010058767,0.00076690345,0.0009760569,0.0029175042,0.0008961999,0.0015487204,0.001399279,0.0038044525,0.034421124],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000496017,0.000016659309,0.0010968265,0.00013369272,0.000020477955,0.00021479296,0.000033720775,0.00005708173,0.0003480486,0.0003158719,0.9887166,0.008996572],"study_design_scores_gemma":[0.00002390504,0.000047960486,0.013536931,0.0002150861,0.00005783688,0.00045078326,0.0001567947,0.00015662328,0.0011303449,0.0003727123,0.9837937,0.00005727274],"about_ca_topic_score_codex":0.028747952,"about_ca_topic_score_gemma":0.03540305,"teacher_disagreement_score":0.040318087,"about_ca_system_score_codex":0.0017898185,"about_ca_system_score_gemma":0.0022503769,"threshold_uncertainty_score":0.1348775},"labels":[],"label_agreement":null},{"id":"W2318885766","doi":"10.3847/0004-637x/826/1/86","title":"PSR J1024–0719: A MILLISECOND PULSAR IN AN UNUSUAL LONG-PERIOD ORBIT","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"Office of Naval Research; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Millisecond pulsar; Astrophysics; Globular cluster; Pulsar; Metallicity; Astronomy; Orbital period; Orbit (dynamics); Halo; Period (music); Stars; Galaxy","score_opus":0.013210866206947783,"score_gpt":0.31993642267304645,"score_spread":0.30672555646609867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2318885766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964857,0.00021784558,0.0003124341,0.00027154997,0.00009053259,0.000011799722,0.00028399497,0.000059359696,0.002266742],"genre_scores_gemma":[0.9979358,0.00007276842,0.0003864316,0.00015967723,0.00010812877,0.0000064672545,0.0005454298,0.000018449675,0.00076701294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991715,0.0000072874896,0.0000073157685,0.000022290533,0.000019544283,0.000026481925],"domain_scores_gemma":[0.9997727,0.000017148255,0.00007252298,0.000016911852,0.000016786116,0.00010386803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011404721,0.00032180818,0.00039036974,0.0006381615,0.00085400214,0.0006471302,0.00043593487,0.00059927476,0.0017340082],"category_scores_gemma":[0.00022537465,0.00014236302,0.0002008823,0.00067191786,0.00048216258,0.00031946358,0.0005759078,0.00058803736,0.00091962726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010022955,0.0008238653,0.6013711,0.00014298076,0.00021522166,0.10910462,0.00047976465,0.00080739654,0.24082534,0.0028758522,0.008991673,0.033359896],"study_design_scores_gemma":[0.00022174783,0.00095483084,0.8840851,0.000023709923,0.00010154254,0.07560662,0.0005498394,0.0020346902,0.016193366,0.0015706989,0.01860297,0.00005484217],"about_ca_topic_score_codex":0.001332225,"about_ca_topic_score_gemma":0.0015847008,"teacher_disagreement_score":0.0017340082,"about_ca_system_score_codex":0.00046405752,"about_ca_system_score_gemma":0.00015743806,"threshold_uncertainty_score":0.0058008432},"labels":[],"label_agreement":null},{"id":"W2319037637","doi":"10.1086/519726","title":"10 Years of<i>RXTE</i>Monitoring of the Anomalous X‐Ray Pulsar 4U 0142+61: Long‐Term Variability","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Magnetar; Glitch; Astrophysics; Flux (metallurgy); Astronomy; X-ray pulsar; Phase (matter); Detector; Optics","score_opus":0.011137326826044385,"score_gpt":0.2408925331322652,"score_spread":0.22975520630622082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2319037637","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99712723,0.0002685366,0.0005930665,0.00008293938,0.000014527003,0.000012527969,0.00051660166,0.000043288423,0.0013413909],"genre_scores_gemma":[0.9956298,0.00015566923,0.0008853231,0.00010259723,0.00005678523,0.000016331329,0.002642415,0.000012034527,0.0004991047],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996847,0.000035161636,0.00003107238,0.000100350626,0.000078134064,0.00007053757],"domain_scores_gemma":[0.9988304,0.0001639387,0.0004381524,0.00013617476,0.00021302748,0.00021835689],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008119777,0.0003092212,0.00040800424,0.0007583856,0.0007049791,0.0007030717,0.00032781457,0.00072175055,0.00042059307],"category_scores_gemma":[0.000969909,0.00016623506,0.00028402384,0.00054773665,0.00035538746,0.00058124954,0.0013122763,0.00058142573,0.00027464158],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054476806,0.00041513072,0.9004861,0.00013124228,0.00037647382,0.002366669,0.0013341855,0.0024064574,0.04163243,0.0003063831,0.0014042392,0.048595946],"study_design_scores_gemma":[0.00001028363,0.0004552454,0.9894527,0.00002015635,0.0000851388,0.00094716024,0.00019666957,0.000885768,0.0030145175,0.00010006415,0.004809833,0.00002244738],"about_ca_topic_score_codex":0.0025170173,"about_ca_topic_score_gemma":0.004926962,"teacher_disagreement_score":0.0025170173,"about_ca_system_score_codex":0.00028998218,"about_ca_system_score_gemma":0.000177428,"threshold_uncertainty_score":0.0050047636},"labels":[],"label_agreement":null},{"id":"W2320633289","doi":"10.1088/0004-637x/753/2/180","title":"ERRATUM: “THE FIRST SYSTEMATIC STUDY OF TYPE Ibc SUPERNOVA MULTI-BAND LIGHT CURVES” (2011, ApJ, 741, 97)","year":2012,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Relativity and Gravitational Theory","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Supernova; Light curve; Astrophysics; Astronomy","score_opus":0.023714489986854527,"score_gpt":0.2629334374907974,"score_spread":0.23921894750394287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2320633289","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0015437463,0.0019805979,0.0006125348,0.030061841,0.9511863,0.00003886706,0.005982881,0.00054142636,0.008051741],"genre_scores_gemma":[0.034267366,0.011137225,0.0080852285,0.09232107,0.26090336,0.00027922235,0.029055102,0.0030976604,0.5608538],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9984627,0.00014957268,0.00040503306,0.00024449886,0.00058474246,0.00015339667],"domain_scores_gemma":[0.9900064,0.001966321,0.00076622627,0.00081881415,0.0059168283,0.0005255577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016174013,0.002183721,0.0013452676,0.0042170896,0.0032734538,0.0022646012,0.002319611,0.0032676558,0.044148084],"category_scores_gemma":[0.020059656,0.00079842826,0.0012520881,0.0022564726,0.001127196,0.0019927106,0.0017145086,0.0037876954,0.032247614],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005844635,0.000013143075,0.00034872943,0.00010117614,0.000013765867,0.0002319194,0.000018938812,0.000031448417,0.000120176,0.00029439063,0.99369425,0.005073553],"study_design_scores_gemma":[0.000047888705,0.00006730045,0.00832069,0.0004153792,0.00009541933,0.0008991511,0.00015957498,0.00020424768,0.0009889341,0.0009829324,0.98775,0.000068403635],"about_ca_topic_score_codex":0.019359687,"about_ca_topic_score_gemma":0.03012023,"teacher_disagreement_score":0.044148084,"about_ca_system_score_codex":0.0023039607,"about_ca_system_score_gemma":0.003007132,"threshold_uncertainty_score":0.14769006},"labels":[],"label_agreement":null},{"id":"W2323061113","doi":"10.1086/322297","title":"White Dwarfs in the Calan‐ESO Survey","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Brown dwarf; Balmer series; Astrophysics; Proper motion; Massive compact halo object; Stars; Sky; Atmosphere (unit); Astronomy; Blue dwarf; Black dwarf; Spectral line; Emission spectrum; Meteorology","score_opus":0.018694866456288865,"score_gpt":0.2415011728816474,"score_spread":0.22280630642535854,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2323061113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99481356,0.00022717039,0.00006598847,0.000037070226,0.000003761737,0.000009710862,0.0029297096,0.000010039663,0.0019028663],"genre_scores_gemma":[0.98139876,0.00046760647,0.0004580228,0.00009063936,0.000012388205,0.000022455257,0.014473994,0.000009300537,0.0030668196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975795,0.000012439522,0.000012721698,0.00006725588,0.00008059723,0.000068984955],"domain_scores_gemma":[0.99972767,0.000019531339,0.00007509939,0.000031476004,0.0000623392,0.00008387344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002886103,0.00022216649,0.00021603015,0.0014888445,0.00059183384,0.00046877828,0.00022059838,0.00015977962,0.0011137617],"category_scores_gemma":[0.0004784398,0.00011518792,0.00009390202,0.0013813752,0.00014258255,0.00020480467,0.0004398383,0.00015170025,0.00038817732],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008629785,0.000035415655,0.9845596,0.000019958978,0.000022907447,0.00015420845,0.00048178702,0.00006784716,0.0025772958,0.0002721135,0.0028295154,0.008893112],"study_design_scores_gemma":[0.0000033276644,0.0000057179404,0.99641633,0.000002224623,0.000004340681,0.000054802967,0.000115790506,0.000045087818,0.000100562655,0.0000108112245,0.0032400163,9.1741197e-7],"about_ca_topic_score_codex":0.0870756,"about_ca_topic_score_gemma":0.21564317,"teacher_disagreement_score":0.0870756,"about_ca_system_score_codex":0.0005670505,"about_ca_system_score_gemma":0.00053322146,"threshold_uncertainty_score":0.17313749},"labels":[],"label_agreement":null},{"id":"W2323094335","doi":"10.3847/1538-4357/833/2/177","title":"THE REPEATING FAST RADIO BURST FRB 121102: MULTI-WAVELENGTH OBSERVATIONS AND ADDITIONAL BURSTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":310,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University; McGill University Health Centre","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Fast radio burst; Jansky; Green Bank Telescope; Sky; Galactic Center; Telescope; Radio telescope; Astronomy; Neutron star; Galaxy; Radio galaxy","score_opus":0.023858242085710992,"score_gpt":0.2952568710475255,"score_spread":0.27139862896181455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2323094335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960647,0.0002751353,0.0005425116,0.00007021797,0.00002503718,0.000015242983,0.00072345854,0.0001284904,0.0021551352],"genre_scores_gemma":[0.9936592,0.00012599143,0.001357227,0.000082464474,0.00008048139,0.000015602236,0.0037401936,0.00003472197,0.000904183],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995746,0.00003666195,0.000034048204,0.000109705994,0.00013753788,0.00010740726],"domain_scores_gemma":[0.99825007,0.00025082505,0.0006444113,0.00024532096,0.00016139747,0.00044796625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004225824,0.0005635222,0.00056896516,0.0018242213,0.00051189086,0.00081623386,0.00052908773,0.0007688635,0.0022983558],"category_scores_gemma":[0.00096376904,0.00030695484,0.00039119076,0.0011378884,0.00021609443,0.00035474193,0.000623768,0.0005510474,0.0008405241],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010325804,0.00049629126,0.80216545,0.00017703846,0.00019461624,0.0039854306,0.00063991686,0.0011889512,0.1346716,0.00019506425,0.0028793993,0.052373737],"study_design_scores_gemma":[0.000024446335,0.00019960845,0.9919926,0.000017845487,0.000028361976,0.0016923426,0.00007910738,0.0008006332,0.0025115763,0.00004914682,0.0025798816,0.000024450603],"about_ca_topic_score_codex":0.0031966479,"about_ca_topic_score_gemma":0.0058102785,"teacher_disagreement_score":0.0031966479,"about_ca_system_score_codex":0.0003476534,"about_ca_system_score_gemma":0.00015179532,"threshold_uncertainty_score":0.0076887608},"labels":[],"label_agreement":null},{"id":"W2323584535","doi":"10.3847/0004-637x/821/1/53","title":"A SUBSTRUCTURE INSIDE SPIRAL ARMS, AND A MIRROR IMAGE ACROSS THE GALACTIC MERIDIAN","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Substructure; Offset (computer science); Milky Way; Meridian (astronomy); Spiral galaxy; Galactic tide; Galactic Center","score_opus":0.009592027002390882,"score_gpt":0.2544504881278978,"score_spread":0.2448584611255069,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2323584535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99074006,0.00023914443,0.0013962114,0.00009469695,0.000016601321,0.0000050354383,0.000088069755,0.00010767721,0.0073124687],"genre_scores_gemma":[0.9977581,0.000038895418,0.0010474029,0.000019806757,0.0000070284937,0.0000016366355,0.00005810498,0.0000075508137,0.0010614663],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999517,0.0000035606065,0.0000025233148,0.000017681832,0.000013377455,0.000011148516],"domain_scores_gemma":[0.9997003,0.000033081375,0.000097809854,0.00008036233,0.00004918939,0.000039166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000051768737,0.00013803397,0.000098200486,0.00039933337,0.00035850992,0.0008249741,0.00020882735,0.0002668155,0.0025290705],"category_scores_gemma":[0.00028312168,0.00014130096,0.00012840562,0.00029728567,0.00052721176,0.0003179695,0.0004189574,0.00032543213,0.00034934297],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010576381,0.00008840476,0.26777217,0.00013408918,0.000084485146,0.005029361,0.0018881034,0.0019783266,0.6439723,0.01482901,0.0014739427,0.0616922],"study_design_scores_gemma":[0.000092299255,0.00042078382,0.8885312,0.00008576612,0.0000865056,0.010319681,0.0012906081,0.0056360583,0.06387286,0.009801879,0.019817391,0.000044833083],"about_ca_topic_score_codex":0.0016102998,"about_ca_topic_score_gemma":0.0012874772,"teacher_disagreement_score":0.0025290705,"about_ca_system_score_codex":0.00022483678,"about_ca_system_score_gemma":0.000088948254,"threshold_uncertainty_score":0.008460641},"labels":[],"label_agreement":null},{"id":"W2323716974","doi":"10.1088/0004-637x/778/1/85","title":"ERRATUM: “STRUCTURE AND DYNAMICS OF THE GLOBULAR CLUSTER PALOMAR 13” (2011, ApJ, 743, 167)","year":2013,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Maritime and Coastal Archaeology","field":"Arts and Humanities","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Astronomy; Galaxy","score_opus":0.005969875175667416,"score_gpt":0.18233417969326948,"score_spread":0.17636430451760207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2323716974","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011812263,0.0007238062,0.00032998683,0.054664847,0.92412305,0.00003478709,0.004357825,0.00055395684,0.014030447],"genre_scores_gemma":[0.022866348,0.00444174,0.0029008687,0.05982181,0.19621715,0.00019114044,0.019749295,0.0034059656,0.6904057],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.998401,0.00013904345,0.000252912,0.00023406112,0.0008098535,0.00016316415],"domain_scores_gemma":[0.9866471,0.0017824131,0.00069235975,0.0008986946,0.009072976,0.0009063722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016374338,0.001607146,0.0012627917,0.003750076,0.006148523,0.0038603789,0.0024314402,0.003906419,0.08507169],"category_scores_gemma":[0.022907134,0.00084623066,0.0012345556,0.002509233,0.0015307815,0.0026631597,0.0022562528,0.005169702,0.053956058],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002738472,0.0000050714834,0.00013410338,0.000034344135,0.000004060477,0.00010780516,0.000014177324,0.000021957725,0.000048946506,0.00023237642,0.99774265,0.0016271521],"study_design_scores_gemma":[0.00004537526,0.000038264458,0.006236386,0.00022720108,0.00005130332,0.0002798886,0.0002801944,0.00026098013,0.00061085087,0.0012144537,0.9906882,0.00006684301],"about_ca_topic_score_codex":0.039429136,"about_ca_topic_score_gemma":0.05094103,"teacher_disagreement_score":0.08507169,"about_ca_system_score_codex":0.0038815718,"about_ca_system_score_gemma":0.005198807,"threshold_uncertainty_score":0.2845931},"labels":[],"label_agreement":null},{"id":"W2324260255","doi":"10.1088/0004-637x/812/2/106","title":"THE C(<sup>3</sup>P) + NH<sub>3</sub>REACTION IN INTERSTELLAR CHEMISTRY. I. INVESTIGATION OF THE PRODUCT FORMATION CHANNELS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Chemical Physics Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Agence Nationale de la Recherche","keywords":"Photoionization; Chemistry; Interstellar cloud; Yield (engineering); Chemical kinetics; Reaction rate constant; Photodissociation; Mass spectrometry; Analytical Chemistry (journal); Photochemistry; Atomic physics; Ionization; Kinetics; Interstellar medium; Ion; Materials science; Physics","score_opus":0.013757062934177491,"score_gpt":0.22050006006584313,"score_spread":0.20674299713166563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2324260255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99006784,0.0012073013,0.005532499,0.00007237903,0.000011974307,0.000021715095,0.00006688025,0.000066838686,0.002952649],"genre_scores_gemma":[0.9952017,0.00042527542,0.003665696,0.000016973541,0.000003259557,0.000010471115,0.000053287284,0.000004588141,0.0006186785],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99993896,0.000011469204,0.0000013729962,0.000013484903,0.000021743397,0.000012909779],"domain_scores_gemma":[0.9999107,0.000044692417,0.00001969211,0.0000070525903,0.000008361622,0.000009578112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013366921,0.0002558232,0.0001219767,0.00010416098,0.00028127976,0.0002035758,0.0003224817,0.00043004824,0.0006894161],"category_scores_gemma":[0.00020396068,0.00009794573,0.00016043012,0.00008813206,0.00044013213,0.0003683499,0.00018805994,0.00023939979,0.00012982987],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005450613,0.00010730653,0.0071583856,0.00037589672,0.000031340278,0.0005794851,0.000098749115,0.017826883,0.9539601,0.005229994,0.00024578383,0.013840917],"study_design_scores_gemma":[0.000032620657,0.0005350941,0.014468478,0.000010640905,0.000026339332,0.0005731438,0.000076221055,0.046125345,0.93329066,0.0021113195,0.002735465,0.000014573259],"about_ca_topic_score_codex":0.0011644579,"about_ca_topic_score_gemma":0.0012511178,"teacher_disagreement_score":0.0011644579,"about_ca_system_score_codex":0.0005840991,"about_ca_system_score_gemma":0.00022141321,"threshold_uncertainty_score":0.00423795},"labels":[],"label_agreement":null},{"id":"W2324298055","doi":"10.3847/0004-637x/821/1/37","title":"THE DIVERSE ORIGINS OF NEUTRON-CAPTURE ELEMENTS IN THE METAL-POOR STAR HD 94028: POSSIBLE DETECTION OF PRODUCTS OF i-PROCESS NUCLEOSYNTHESIS*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Canadian Space Agency; National Institute of Standards and Technology; Magyar Tudományos Akadémia; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Texas at Austin; European Southern Observatory; Space Telescope Science Institute; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; National Science Foundation; Compute Canada; Canarie; Canadian Foundation for AIDS Research; National Aeronautics and Space Administration","keywords":"Stars; Nucleosynthesis; Space Telescope Imaging Spectrograph; Spectrograph; Carbon star; Spitzer Space Telescope; r-process; Star (game theory)","score_opus":0.011980555566326545,"score_gpt":0.2299895292195393,"score_spread":0.21800897365321276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2324298055","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991449,0.00006523849,0.00018159034,0.0000039609304,5.7685656e-7,0.000002444397,0.00011869143,0.000009293529,0.0004731988],"genre_scores_gemma":[0.9990219,0.000030081612,0.00041155232,0.000007668445,0.0000016613997,0.0000038961125,0.00031609414,0.000004410224,0.00020273714],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993265,0.0000069349317,0.000006265296,0.000022989916,0.000018291788,0.0000129211385],"domain_scores_gemma":[0.9998252,0.000030376781,0.000056026613,0.000021028081,0.000032762913,0.000034610744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017166155,0.0002904426,0.00024470294,0.0010692725,0.00033183367,0.000378772,0.0002876047,0.00022084248,0.00071741897],"category_scores_gemma":[0.00021774364,0.0001528011,0.00016003686,0.0004723933,0.00021559681,0.00016398942,0.00032453766,0.0001250851,0.00019850684],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059629604,0.00005119278,0.7209467,0.000053725806,0.00006298987,0.00020443276,0.00014021277,0.00047803068,0.27120292,0.00022425158,0.00008572433,0.00595357],"study_design_scores_gemma":[0.000017886228,0.00015176073,0.9727762,0.00000636553,0.000031415715,0.00029412657,0.00013227317,0.0017430113,0.02376841,0.00014900252,0.00092301675,0.0000064196292],"about_ca_topic_score_codex":0.002081742,"about_ca_topic_score_gemma":0.0028560385,"teacher_disagreement_score":0.002081742,"about_ca_system_score_codex":0.0003132776,"about_ca_system_score_gemma":0.000055682885,"threshold_uncertainty_score":0.0041392446},"labels":[],"label_agreement":null},{"id":"W2324462846","doi":"10.3847/0004-637x/824/1/11","title":"SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT. IV. ANOMALOUS BEHAVIOR OF THE BROAD ULTRAVIOLET EMISSION LINES IN NGC 5548","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Natural Sciences and Engineering Research Council of Canada; University of California, Santa Barbara; Jet Propulsion Laboratory; National Research Foundation of Korea; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Space Telescope Science Institute; American Academy in Rome; Science and Technology Facilities Council; National Research Foundation; David and Lucile Packard Foundation; Ministry of Science, ICT and Future Planning; Ohio State University; Howard Hughes Medical Institute; Danmarks Grundforskningsfond; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Georgia State University; California Institute of Technology; National Aeronautics and Space Administration; Danmarks Frie Forskningsfond; National Science Foundation","keywords":"Space Telescope Imaging Spectrograph; Emission spectrum; Active galactic nucleus; Reverberation mapping; Galaxy; Flux (metallurgy); Spectral line; Spitzer Space Telescope; Spectral energy distribution; Photon","score_opus":0.00891891466956792,"score_gpt":0.22630579247397611,"score_spread":0.21738687780440819,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2324462846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9934442,0.00005863959,0.00062927324,0.000059906484,0.00001229326,0.00002422935,0.0034323523,0.000120294346,0.0022188083],"genre_scores_gemma":[0.98500776,0.000048009828,0.002517466,0.000034187287,0.000013148146,0.000024142078,0.009833516,0.000031611624,0.0024901365],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998591,0.000017848626,0.0000055404416,0.000037106332,0.000037157748,0.00004320721],"domain_scores_gemma":[0.9996183,0.000019930054,0.00009243951,0.00008769049,0.0000923359,0.0000892116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032445567,0.00021700124,0.000116860385,0.0007668246,0.00028342227,0.00030016672,0.00023110682,0.00014764728,0.0016467621],"category_scores_gemma":[0.00042632592,0.00007991986,0.00010930994,0.00040857948,0.0001130914,0.00019839311,0.0003020211,0.00015009008,0.00070087746],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051837496,0.0002057609,0.89608705,0.000028251805,0.000057316855,0.0005918327,0.0007230824,0.0009077558,0.04317105,0.00023703021,0.004571523,0.05290087],"study_design_scores_gemma":[0.0000094198895,0.0000822827,0.9924177,0.0000029088183,0.000010296422,0.00015022919,0.000111649264,0.0006971026,0.0024064996,0.000032618085,0.004075663,0.000003706528],"about_ca_topic_score_codex":0.015883882,"about_ca_topic_score_gemma":0.026601769,"teacher_disagreement_score":0.015883882,"about_ca_system_score_codex":0.00028375592,"about_ca_system_score_gemma":0.00016553578,"threshold_uncertainty_score":0.031582892},"labels":[],"label_agreement":null},{"id":"W2329129041","doi":"10.3847/0004-637x/821/1/9","title":"THE ATMOSPHERIC CIRCULATION OF A NINE-HOT-JUPITER SAMPLE: PROBING CIRCULATION AND CHEMISTRY OVER A WIDE PHASE SPACE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":183,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Hot Jupiter; Planet; Astrophysics; Physics; Exoplanet; Atmospheric sciences","score_opus":0.006291147954469436,"score_gpt":0.21711379453865687,"score_spread":0.21082264658418742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2329129041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992939,0.000009361922,0.00013231876,0.0000123165555,9.735911e-7,0.0000036498964,0.00041111355,0.000012583373,0.00012378313],"genre_scores_gemma":[0.99830073,0.000011085872,0.0003625219,0.000008870228,0.0000044442704,0.0000063170455,0.0011910028,0.000007979913,0.000107105785],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999379,0.000011566114,0.0000033445533,0.000020697318,0.000011062976,0.000015367788],"domain_scores_gemma":[0.99978834,0.000034123168,0.000046084537,0.000037750448,0.000024065084,0.00006958803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013681491,0.00015871429,0.00026423155,0.00039663736,0.00044372494,0.0002958138,0.00023191515,0.00018007917,0.00061335263],"category_scores_gemma":[0.00031907004,0.00011191926,0.00027492738,0.00045901703,0.00020606478,0.00023359532,0.00037174195,0.00025491187,0.00013580447],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006252262,0.00026586518,0.9502056,0.000019140432,0.00014516259,0.00024660843,0.000713823,0.0032937552,0.03554869,0.0001885281,0.000827984,0.007919565],"study_design_scores_gemma":[0.00001963424,0.00008708891,0.9930703,0.0000012725275,0.000023778966,0.00007811626,0.00016315706,0.004396941,0.0015501407,0.000052942625,0.0005498226,0.0000068165828],"about_ca_topic_score_codex":0.012239643,"about_ca_topic_score_gemma":0.011547091,"teacher_disagreement_score":0.012239643,"about_ca_system_score_codex":0.000278704,"about_ca_system_score_gemma":0.000120709934,"threshold_uncertainty_score":0.024336755},"labels":[],"label_agreement":null},{"id":"W2332147304","doi":"10.3847/0004-637x/823/2/117","title":"A SURVEY OF CHEMICAL SEPARATION IN ACCRETING NEUTRON STARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Chemical composition; Stars; Neutron star; Hydrogen; Helium; Range (aeronautics); Convection; Abundance of the chemical elements; Dispersion (optics); Accretion (finance)","score_opus":0.017072618368215876,"score_gpt":0.273673860896525,"score_spread":0.2566012425283091,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2332147304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99681634,0.000768779,0.00059978897,0.0000117448535,0.0000011914647,0.0000036995825,0.00016927718,0.0000184898,0.0016107417],"genre_scores_gemma":[0.9983448,0.0004547144,0.0005135267,0.0000060857665,0.0000022574295,0.0000014936658,0.0003984072,0.0000065640056,0.0002720078],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997944,0.00003340164,0.000016961452,0.000050738858,0.000078629964,0.000025827092],"domain_scores_gemma":[0.99954283,0.00012619111,0.00015805554,0.000026094729,0.00008795925,0.00005896767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003996855,0.00026482728,0.00030327772,0.0021563363,0.00033667166,0.00051295443,0.00028538893,0.00035196083,0.0006442306],"category_scores_gemma":[0.0007641157,0.00016377222,0.00021542048,0.0012664861,0.00022796831,0.00039560365,0.0004468918,0.00015030806,0.00018482386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005714138,0.00012464647,0.89073014,0.00017814574,0.00016301428,0.00042908604,0.00020355187,0.016313208,0.056450676,0.0017685408,0.00023121125,0.032836396],"study_design_scores_gemma":[0.000019058865,0.00037328564,0.9157955,0.000030610452,0.00005374808,0.0009926904,0.00031057576,0.031653047,0.042792644,0.0013309534,0.0066163526,0.000031563344],"about_ca_topic_score_codex":0.0021063325,"about_ca_topic_score_gemma":0.0012441647,"teacher_disagreement_score":0.0021563363,"about_ca_system_score_codex":0.00035427386,"about_ca_system_score_gemma":0.00016265186,"threshold_uncertainty_score":0.0041881204},"labels":[],"label_agreement":null},{"id":"W2332776368","doi":"10.3847/0004-637x/820/2/144","title":"ERRATUM: “BROADBAND RADIO POLARIMETRY AND FARADAY ROTATION OF 563 EXTRAGALACTIC RADIO SOURCES” (ApJ, 815, 1, 49)","year":2016,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Opinion Dynamics and Social Influence","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Faraday effect; Polarimetry; Broadband; Astrophysics; Astronomy; Faraday cage; Optics; Magnetic field; Scattering; Quantum mechanics","score_opus":0.007623919035313056,"score_gpt":0.24420986600220274,"score_spread":0.23658594696688967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2332776368","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0012394402,0.0011886104,0.0003171994,0.037482165,0.9431517,0.000032395088,0.00586695,0.00037660202,0.010344959],"genre_scores_gemma":[0.02291908,0.007096058,0.0036971946,0.063490644,0.2114986,0.000212016,0.026054254,0.0016973886,0.6633348],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99857104,0.00011924289,0.0004045211,0.000196318,0.0005808913,0.00012803744],"domain_scores_gemma":[0.99189866,0.0013131882,0.00064639054,0.0006922081,0.004897701,0.000551826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014541923,0.002362508,0.0012333068,0.003896262,0.0037507014,0.0026682257,0.0021656961,0.0028327089,0.055821206],"category_scores_gemma":[0.018063042,0.00082061335,0.0013477068,0.002564325,0.0011709377,0.002213777,0.0019427496,0.0039979173,0.044641808],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041207622,0.000012382168,0.000341925,0.00004866668,0.0000066232674,0.0001747101,0.000020255218,0.000032040847,0.00007514696,0.0002707442,0.9954066,0.0035697005],"study_design_scores_gemma":[0.00004830674,0.000048769263,0.008307102,0.00025728252,0.000055967696,0.00041496952,0.00024936916,0.00020523838,0.00064376974,0.0013724705,0.9883415,0.00005519903],"about_ca_topic_score_codex":0.031120582,"about_ca_topic_score_gemma":0.04421251,"teacher_disagreement_score":0.055821206,"about_ca_system_score_codex":0.002799758,"about_ca_system_score_gemma":0.004438986,"threshold_uncertainty_score":0.18674058},"labels":[],"label_agreement":null},{"id":"W2334388385","doi":"10.3847/0004-637x/829/2/132","title":"WARM JUPITERS FROM SECULAR PLANET–PLANET INTERACTIONS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Hot Jupiter; Eccentricity (behavior); Planet; Population; Planetary system; Outer planets","score_opus":0.00916965248302913,"score_gpt":0.21719223260737908,"score_spread":0.20802258012434996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2334388385","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978399,0.00007498726,0.00078903825,0.000029967496,0.000001526656,0.0000040806603,0.000110322886,0.000028473301,0.0011215381],"genre_scores_gemma":[0.99952006,0.000020743215,0.00008605855,0.0000059051504,0.0000017544913,0.000001815281,0.00014543317,0.0000028858392,0.00021533246],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998043,0.00004118862,0.0000070806013,0.000068042165,0.000022780427,0.00005662642],"domain_scores_gemma":[0.99935716,0.00017219846,0.0002091306,0.00011519708,0.000035380897,0.00011099238],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027578272,0.00032779112,0.00042911337,0.000668172,0.00044082556,0.0009909426,0.00045186077,0.0003897149,0.0037198383],"category_scores_gemma":[0.0013024025,0.00020807842,0.00033347934,0.0006152141,0.00053552527,0.0004954639,0.0007476791,0.00033349812,0.00041859114],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014313277,0.00014483703,0.8560232,0.0001149688,0.00028974024,0.0024234564,0.00090310257,0.073580556,0.024600685,0.0052228477,0.0023454407,0.032919936],"study_design_scores_gemma":[0.000065179935,0.0002995386,0.88372505,0.000021878564,0.00011847083,0.0017992512,0.00048823527,0.09877413,0.003956188,0.008119468,0.0026024738,0.000030061261],"about_ca_topic_score_codex":0.002760971,"about_ca_topic_score_gemma":0.0032600653,"teacher_disagreement_score":0.0037198383,"about_ca_system_score_codex":0.0004961499,"about_ca_system_score_gemma":0.00015549171,"threshold_uncertainty_score":0.012444079},"labels":[],"label_agreement":null},{"id":"W2336953531","doi":"10.3847/0004-637x/825/2/98","title":"WARM JUPITERS ARE LESS LONELY THAN HOT JUPITERS: CLOSE NEIGHBORS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":202,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"","keywords":"Hot Jupiter; Planetary system; Population; Transit (satellite); Orbital elements","score_opus":0.015741291897430943,"score_gpt":0.22457504713586204,"score_spread":0.2088337552384311,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2336953531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985189,0.0001373715,0.00013211908,0.000032129996,0.0000050063773,0.0000017450517,0.00013777784,0.000005640961,0.0010293513],"genre_scores_gemma":[0.9995253,0.000026536178,0.000045161,0.000008370925,0.000005329491,9.489476e-7,0.00010958452,0.0000018588372,0.00027680304],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988675,0.000014338861,0.000006391817,0.000052762774,0.000016099566,0.000023609062],"domain_scores_gemma":[0.9989945,0.00022111637,0.00038028488,0.0000814631,0.000072561685,0.00025017085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012305254,0.000099207675,0.00018397972,0.00060374016,0.0004245356,0.0007270839,0.00020155247,0.00016977363,0.009323001],"category_scores_gemma":[0.0012849523,0.000082853665,0.000076508644,0.000477021,0.0002933306,0.0004432472,0.0004138403,0.0002476913,0.0007386407],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001684465,0.000024839746,0.98406845,0.00003087965,0.00007885898,0.00022656341,0.0007717833,0.000056552228,0.0051229373,0.00032347415,0.00062016957,0.008507013],"study_design_scores_gemma":[0.0000021820922,0.000029454231,0.9972663,0.0000048473235,0.00001625879,0.00046799085,0.000802116,0.000093576076,0.00025871335,0.00015353889,0.0009025471,0.0000025515355],"about_ca_topic_score_codex":0.001291291,"about_ca_topic_score_gemma":0.0015284678,"teacher_disagreement_score":0.009323001,"about_ca_system_score_codex":0.000080254365,"about_ca_system_score_gemma":0.0000496261,"threshold_uncertainty_score":0.031188548},"labels":[],"label_agreement":null},{"id":"W2337031390","doi":"10.3847/0004-637x/826/2/167","title":"THE MASSIVE SURVEY. IV. THE X-RAY HALOS OF THE MOST MASSIVE EARLY-TYPE GALAXIES IN THE NEARBY UNIVERSE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Halo; Elliptical galaxy; Velocity dispersion; Astronomy; Stellar mass; Lenticular galaxy; Luminosity; Radio galaxy; Star formation","score_opus":0.00880121609061513,"score_gpt":0.20569547886034725,"score_spread":0.19689426276973213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2337031390","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974833,0.00020408396,0.000102689955,0.00002084616,0.0000017776852,0.0000048073225,0.0013953304,0.00001793877,0.0007691892],"genre_scores_gemma":[0.99679726,0.00009739663,0.00029338402,0.000021733164,0.000007197892,0.0000040894092,0.0021566474,0.0000063563352,0.0006160158],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998087,0.00003307477,0.000014415233,0.000055639444,0.000035130335,0.00005300472],"domain_scores_gemma":[0.99914956,0.0000459612,0.00034494148,0.00010813378,0.000063868996,0.00028752608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048644643,0.00029672842,0.00020799987,0.0014709423,0.00033997674,0.0006305682,0.0002747652,0.00016264518,0.0019620117],"category_scores_gemma":[0.00055495044,0.00016959452,0.00031068336,0.0008699512,0.00022659419,0.0002948992,0.0009956649,0.00016499778,0.0005643562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008603978,0.000010451814,0.9881384,0.000023760229,0.00005966005,0.000039096176,0.00027640464,0.00006241715,0.0052462663,0.00016986541,0.0004217596,0.005465987],"study_design_scores_gemma":[0.000002150974,0.000015725904,0.99920446,0.0000030950819,0.0000073290944,0.00004911527,0.000063168365,0.000036501144,0.00018662645,0.000020542431,0.0004101876,0.000001221581],"about_ca_topic_score_codex":0.0042236526,"about_ca_topic_score_gemma":0.011427397,"teacher_disagreement_score":0.0042236526,"about_ca_system_score_codex":0.00022676862,"about_ca_system_score_gemma":0.00012807388,"threshold_uncertainty_score":0.008398116},"labels":[],"label_agreement":null},{"id":"W2338431697","doi":"10.3847/0004-637x/823/2/87","title":"THE DENSE GAS IN THE LARGEST MOLECULAR COMPLEXES OF THE ANTENNAE: HCN AND HCO<sup>+</sup> OBSERVATIONS OF NGC 4038/39 USING ALMA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Science Council; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Milky Way; Spiral galaxy; Molecular cloud; Galaxy; H II region; Spiral (railway)","score_opus":0.02242749596976863,"score_gpt":0.24790768974465846,"score_spread":0.22548019377488984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2338431697","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965449,0.000066512446,0.00010663239,0.000050728187,0.000002633397,0.00000518265,0.0003741766,0.00005721845,0.0027920536],"genre_scores_gemma":[0.9987557,0.000024823581,0.00029316783,0.000034096898,0.0000061210308,0.0000067885708,0.00033260114,0.000013174768,0.0005334792],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989307,0.0000036982262,0.00000300863,0.000036750273,0.00003171929,0.000031807256],"domain_scores_gemma":[0.9998745,0.000009249878,0.00003138165,0.00001446325,0.000013877848,0.000056647572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000103230304,0.0002746688,0.00024267042,0.000791455,0.00056654,0.00047501337,0.00041807748,0.00023331441,0.00274111],"category_scores_gemma":[0.00014100109,0.00024558246,0.00015212163,0.00046276808,0.00032634928,0.00024547477,0.00054834515,0.00024883836,0.00047884288],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005862949,0.00010220498,0.3985738,0.000058839676,0.00010104461,0.0005557729,0.00093906396,0.00088619784,0.578861,0.0006389463,0.0019405821,0.016756255],"study_design_scores_gemma":[0.000032337764,0.00003617685,0.98364496,0.000008963378,0.00001818845,0.00024420966,0.00021266047,0.0010897082,0.011228478,0.00018122837,0.00328941,0.000013668247],"about_ca_topic_score_codex":0.022614587,"about_ca_topic_score_gemma":0.04601869,"teacher_disagreement_score":0.022614587,"about_ca_system_score_codex":0.0009559751,"about_ca_system_score_gemma":0.0001654045,"threshold_uncertainty_score":0.044965923},"labels":[],"label_agreement":null},{"id":"W2338633135","doi":"10.3847/0004-637x/822/2/95","title":"THE GLOBULAR CLUSTER SYSTEM OF THE COMA CD GALAXY NGC 4874 FROM HUBBLE SPACE TELESCOPE ACS AND WFC3/IR IMAGING*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Advanced Camera for Surveys; Galaxy; Coma Cluster; Metallicity; Astronomy; Photometry (optics); Hubble space telescope; Galaxy cluster; Stars","score_opus":0.003693159215341878,"score_gpt":0.18512326380426222,"score_spread":0.18143010458892034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2338633135","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99534565,0.000059018854,0.00008665287,0.000019421004,0.0000030533008,0.000005540415,0.0021271969,0.000038845843,0.0023146262],"genre_scores_gemma":[0.9972464,0.000030272959,0.00027530413,0.000009976185,0.0000059797176,0.0000035558837,0.0019887856,0.0000052027353,0.000434628],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999198,0.0000035100659,0.0000023957605,0.000019370225,0.000025440128,0.000029530629],"domain_scores_gemma":[0.99982625,0.000008500288,0.00003396129,0.00001933005,0.000052010822,0.00006006321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006336271,0.00015936318,0.00011964146,0.0017269161,0.0004659844,0.00036457615,0.00018902044,0.00010376017,0.0043937485],"category_scores_gemma":[0.00019329369,0.00007740912,0.00010312228,0.0009634753,0.00015341764,0.00017326933,0.00028911897,0.00010066272,0.00063548674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014685252,0.000043090888,0.9646663,0.000019177898,0.000045734258,0.00028907228,0.00016820946,0.0006248465,0.014694021,0.00030249797,0.0039423835,0.015057859],"study_design_scores_gemma":[0.0000015110368,0.0000046285104,0.99843174,0.000001385783,0.0000040966543,0.00004498198,0.00005349236,0.0002960188,0.00029825687,0.000026066615,0.00083595933,0.0000018969445],"about_ca_topic_score_codex":0.08267867,"about_ca_topic_score_gemma":0.14900514,"teacher_disagreement_score":0.08267867,"about_ca_system_score_codex":0.0006917376,"about_ca_system_score_gemma":0.00025539598,"threshold_uncertainty_score":0.16439486},"labels":[],"label_agreement":null},{"id":"W2338729722","doi":"10.3847/0004-637x/826/2/112","title":"ALMA IMAGING AND GRAVITATIONAL LENS MODELS OF SOUTH POLE TELESCOPE—SELECTED DUSTY, STAR-FORMING GALAXIES AT HIGH REDSHIFTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":211,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Gravitational lens; Galaxy; Redshift; Mass distribution; Magnification; Lens (geology); Luminosity; Wavelength; Telescope; South Pole Telescope","score_opus":0.00844043132052981,"score_gpt":0.2013462200624443,"score_spread":0.1929057887419145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2338729722","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99411774,0.00010363424,0.0044338354,0.000079862526,0.0000022002203,0.000006949539,0.00012566343,0.00007057037,0.0010594934],"genre_scores_gemma":[0.9989912,0.000015270167,0.0007251116,0.0000072251846,0.0000032444598,0.0000022464374,0.000087348446,0.0000065402032,0.00016186763],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987197,0.0000304167,0.0000055977775,0.000045254543,0.000024117277,0.000022705553],"domain_scores_gemma":[0.9994561,0.00016440522,0.00019462759,0.00004794134,0.00005886373,0.00007803549],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005263328,0.00035097907,0.00026538485,0.00086609204,0.0003378372,0.00095109147,0.00063418504,0.00044009983,0.0011205075],"category_scores_gemma":[0.0010835128,0.0003088267,0.00054344814,0.00039408036,0.00034054896,0.0006400409,0.00038475028,0.00024258022,0.00023577202],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025829583,0.00007406647,0.6406907,0.000039892617,0.00020595927,0.0002243745,0.0003091128,0.32927564,0.0123741655,0.006100333,0.0007287073,0.00971884],"study_design_scores_gemma":[0.000025065377,0.00004617273,0.212241,0.000006562533,0.000036063968,0.000076345095,0.000072527066,0.7839954,0.001116987,0.0017537666,0.0006156804,0.000014478822],"about_ca_topic_score_codex":0.03379954,"about_ca_topic_score_gemma":0.023831617,"teacher_disagreement_score":0.03379954,"about_ca_system_score_codex":0.0022281585,"about_ca_system_score_gemma":0.00030409914,"threshold_uncertainty_score":0.06720561},"labels":[],"label_agreement":null},{"id":"W2338827753","doi":"10.3847/0004-637x/825/1/59","title":"A STUDY OF BROADBAND FARADAY ROTATION AND POLARIZATION BEHAVIOR OVER 1.3–10 GHz IN 36 DISCRETE RADIO SOURCES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Polarization (electrochemistry); Faraday effect; Broadband; Narrowband; Linear polarization; Faraday cage; Spectral line; Circular polarization","score_opus":0.008457455493386975,"score_gpt":0.236049635601998,"score_spread":0.22759218010861101,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2338827753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979036,0.00008301796,0.0013867406,0.000012240212,0.0000014053232,0.00000451417,0.00022139326,0.000018942883,0.00036823459],"genre_scores_gemma":[0.9977157,0.00007181191,0.0013396902,0.000005075634,0.00001152165,0.000006364292,0.00069360936,0.000012176485,0.00014401645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986184,0.000019663936,0.0000064027854,0.000044727924,0.0000341191,0.000033272652],"domain_scores_gemma":[0.99945253,0.00014700653,0.00016596499,0.000057090307,0.00009938483,0.00007799346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022030936,0.00030863454,0.000346031,0.0023939484,0.00044705093,0.00045169864,0.00022813487,0.00022930176,0.0008444863],"category_scores_gemma":[0.000589708,0.00023908657,0.00030540366,0.0014757132,0.0002613054,0.0003233967,0.0004999023,0.00024905414,0.00033051425],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005576407,0.00017243186,0.74035823,0.00008030949,0.00021056393,0.00063633453,0.0010482471,0.005308523,0.20437221,0.0004391317,0.00035557832,0.04646083],"study_design_scores_gemma":[0.000008701811,0.000046659443,0.99219817,0.0000044834924,0.000030741492,0.00027940774,0.00014337525,0.0028741474,0.0037981952,0.00011961608,0.0004832284,0.000013287862],"about_ca_topic_score_codex":0.0019426561,"about_ca_topic_score_gemma":0.002150189,"teacher_disagreement_score":0.0023939484,"about_ca_system_score_codex":0.00017263574,"about_ca_system_score_gemma":0.00007774081,"threshold_uncertainty_score":0.003862679},"labels":[],"label_agreement":null},{"id":"W2338956948","doi":"10.3847/0004-637x/823/2/160","title":"AN ALMA SEARCH FOR SUBSTRUCTURE, FRAGMENTATION, AND HIDDEN PROTOSTARS IN STARLESS CORES IN CHAMAELEON I","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Astrophysics; Substructure; Physics; Star formation; Fragmentation (computing); Population; Molecular cloud; Turbulence; Astronomy; Stars; Biology","score_opus":0.01347941966076511,"score_gpt":0.2795884147623774,"score_spread":0.2661089951016123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2338956948","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99825865,0.000047610873,0.00018117976,0.00001974179,0.0000014184067,0.000004363978,0.00018655989,0.000015806769,0.0012847203],"genre_scores_gemma":[0.9993236,0.0000109826915,0.00023146941,0.00000891526,0.0000018503305,0.0000020220336,0.00022361154,0.0000024078236,0.00019516864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999231,0.0000072304,0.0000018330564,0.00002856427,0.00001993345,0.000019426103],"domain_scores_gemma":[0.9996568,0.000046420253,0.00011155144,0.000037919028,0.000028467315,0.00011884775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019003895,0.00015845148,0.00014792335,0.0011795587,0.00052447687,0.0004265322,0.00028307823,0.00019106641,0.0021474017],"category_scores_gemma":[0.0003620462,0.00009116367,0.00013802265,0.0004231772,0.00019602016,0.00018435973,0.00042707412,0.0001538479,0.00021732032],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017383746,0.00004192988,0.9515839,0.000015413054,0.00005701838,0.000333208,0.00045968848,0.00067533884,0.038959738,0.00037390483,0.00032593455,0.007000154],"study_design_scores_gemma":[0.0000050943136,0.000029236846,0.99677604,0.0000034739007,0.000007982001,0.0000938657,0.00015153254,0.0009046031,0.0011926325,0.00007064013,0.0007606868,0.000004193026],"about_ca_topic_score_codex":0.014535484,"about_ca_topic_score_gemma":0.041866887,"teacher_disagreement_score":0.014535484,"about_ca_system_score_codex":0.0006175019,"about_ca_system_score_gemma":0.00015298919,"threshold_uncertainty_score":0.028901756},"labels":[],"label_agreement":null},{"id":"W2339495717","doi":"10.3847/0004-637x/824/1/1","title":"THE SECRET LIVES OF CEPHEIDS: EVOLUTION, MASS-LOSS, AND ULTRAVIOLET EMISSION OF THE LONG-PERIOD CLASSICAL CEPHEID*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cepheid variable; Spectrograph; Period (music); Ultraviolet; Stellar evolution; Stellar physics; Stellar pulsation; COSMIC cancer database","score_opus":0.005746250369416004,"score_gpt":0.2067963659843521,"score_spread":0.2010501156149361,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2339495717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99812263,0.00021235037,0.0001283907,0.000074516254,0.0000038389176,0.0000010589521,0.00016078299,0.0000046424993,0.0012918807],"genre_scores_gemma":[0.9996791,0.00004598994,0.00005851034,0.000007777102,0.0000051984543,5.6112526e-7,0.000094947296,0.000001356416,0.00010649536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992204,0.000012569794,0.00000427267,0.000020105026,0.000025567608,0.000015439362],"domain_scores_gemma":[0.99884975,0.00023496337,0.0004978201,0.000069778434,0.00015628248,0.00019133819],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027347176,0.00009708781,0.000104217404,0.000532549,0.0003915327,0.0008141277,0.0001632032,0.00020638843,0.0010590754],"category_scores_gemma":[0.001707422,0.000058214384,0.00006259889,0.00049477746,0.00045520742,0.0005318097,0.00031399072,0.00027951723,0.00016993866],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014264938,0.000038286427,0.97531486,0.000024115878,0.000029469047,0.00014448402,0.0007566939,0.0005342375,0.0050790277,0.001375378,0.0008268134,0.015734058],"study_design_scores_gemma":[9.726629e-7,0.000016785038,0.9980233,0.0000032083724,0.000004191824,0.00006774151,0.00020767307,0.0005879465,0.00032379272,0.00026610144,0.00049502554,0.0000032376215],"about_ca_topic_score_codex":0.0033670238,"about_ca_topic_score_gemma":0.0043142946,"teacher_disagreement_score":0.0033670238,"about_ca_system_score_codex":0.00036230672,"about_ca_system_score_gemma":0.00006810143,"threshold_uncertainty_score":0.0066948533},"labels":[],"label_agreement":null},{"id":"W2340118441","doi":"10.3847/0004-637x/823/1/9","title":"THE ACS LCID PROJECT. XI. ON THE EARLY TIME RESOLUTION OF SFHs OF LOCAL GROUP DWARF GALAXIES: COMPARING THE EFFECTS OF REIONIZATION IN MODELS WITH OBSERVATIONS*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Reionization; Local Group; Dwarf galaxy; Galaxy; Star formation; COSMIC cancer database; Galaxy formation and evolution","score_opus":0.012583130144504321,"score_gpt":0.199635008618645,"score_spread":0.18705187847414068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2340118441","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.082029484,0.002295732,0.016273074,0.0033587932,0.00046250265,0.00026797038,0.7898504,0.023937842,0.08152419],"genre_scores_gemma":[0.26414093,0.0012675892,0.04680515,0.00080287876,0.0002807715,0.0006518857,0.651202,0.0059776236,0.028871182],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994448,0.00012606649,0.000023082277,0.00012257509,0.00022138994,0.00006213728],"domain_scores_gemma":[0.9978946,0.00053510565,0.00018086257,0.00053789595,0.00053786975,0.00031386444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023169396,0.00053992047,0.0006740524,0.0022248684,0.0007819683,0.002412937,0.0018164917,0.00054865045,0.037136972],"category_scores_gemma":[0.004022547,0.0003026342,0.00055647275,0.00315977,0.00023215188,0.0010047398,0.0015130781,0.00042578776,0.01431656],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017947389,0.00023245692,0.10044692,0.0006267386,0.00026296594,0.0002054548,0.0003681593,0.013976203,0.0051214052,0.02329008,0.6900243,0.1636505],"study_design_scores_gemma":[0.0008658591,0.00012436797,0.20188178,0.00027800907,0.00022295302,0.00019561446,0.0003576577,0.13103092,0.008089346,0.017486552,0.63934416,0.00012287815],"about_ca_topic_score_codex":0.09331723,"about_ca_topic_score_gemma":0.060593754,"teacher_disagreement_score":0.09331723,"about_ca_system_score_codex":0.0020021754,"about_ca_system_score_gemma":0.0011501646,"threshold_uncertainty_score":0.18554813},"labels":[],"label_agreement":null},{"id":"W2340513637","doi":"10.3847/0004-637x/823/2/93","title":"A SEARCH FOR SUB-SECOND RADIO VARIABILITY PREDICTED TO ARISE TOWARD 3C 84 FROM INTERGALACTIC DISPERSION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Jansky; Dispersion (optics); Spectral line; Spectral density; Ranging; Electron density; Light curve; Intergalactic travel; Magnitude (astronomy)","score_opus":0.012988927420260728,"score_gpt":0.23675858543608427,"score_spread":0.22376965801582355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2340513637","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99897987,0.000012285826,0.00047557926,0.000021016514,6.5419965e-7,0.000001337684,0.000023503846,0.0000074315603,0.00047837608],"genre_scores_gemma":[0.9998584,0.0000024727453,0.00008883226,0.0000033689262,0.0000010208813,9.3786554e-7,0.000021625863,7.367718e-7,0.000022480734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998658,0.000032911244,0.000004727539,0.000034537694,0.00003507074,0.000026997284],"domain_scores_gemma":[0.9985587,0.0006571294,0.00043274835,0.00012969901,0.00009562941,0.00012614683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004586042,0.00016237865,0.00013157017,0.0007585276,0.00030723066,0.00048990914,0.00030777123,0.000322027,0.0008973564],"category_scores_gemma":[0.0019415858,0.000111896,0.0001606112,0.0003618861,0.00035484307,0.00026374354,0.0003497267,0.00030139636,0.000118827054],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001198931,0.000042998945,0.9803232,0.00000541116,0.00003889806,0.00012787103,0.00006559008,0.0033497256,0.010465034,0.0009954461,0.000121416546,0.0043444876],"study_design_scores_gemma":[0.000008975314,0.00006311355,0.9739005,0.0000026961507,0.000019837755,0.00015135275,0.00007900029,0.023213947,0.0017892306,0.0006006504,0.00016580512,0.000004981618],"about_ca_topic_score_codex":0.0011907036,"about_ca_topic_score_gemma":0.001370084,"teacher_disagreement_score":0.0011907036,"about_ca_system_score_codex":0.00034315913,"about_ca_system_score_gemma":0.00012090139,"threshold_uncertainty_score":0.0030019283},"labels":[],"label_agreement":null},{"id":"W2340645962","doi":"10.3847/0004-637x/830/2/143","title":"MILLIMETER TRANSIENT POINT SOURCES IN THE SPTpol 100 SQUARE DEGREE SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); McGill University; Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Argonne National Laboratory; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of Colorado Boulder; Office of Science; McGill University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Gordon and Betty Moore Foundation; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Transient (computer programming); Millimeter; Square (algebra); Degree (music); Point (geometry); Environmental science; Physics; Mathematics; Computer science; Acoustics; Optics; Geometry","score_opus":0.02849204256310126,"score_gpt":0.24171917984572794,"score_spread":0.21322713728262668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2340645962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99688244,0.00008535401,0.000637418,0.000031263582,0.000002997272,0.000012754227,0.0011369389,0.000055518514,0.0011553366],"genre_scores_gemma":[0.9968093,0.00008183091,0.00059765956,0.000012867765,0.00000592398,0.000012961072,0.0021838483,0.000011067009,0.00028445994],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979883,0.00002815171,0.000009864478,0.000052924992,0.000059652895,0.000050482697],"domain_scores_gemma":[0.99957174,0.00006081586,0.00015201754,0.000073098076,0.000060530943,0.000081803286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021079821,0.00017880142,0.00018590642,0.0011306211,0.00022363225,0.0006533515,0.0002836388,0.0002078924,0.0011158542],"category_scores_gemma":[0.00043582995,0.00019493,0.00018030802,0.001730349,0.00024839322,0.00039780198,0.0008232826,0.00029676972,0.0005503739],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000195707,0.00005983658,0.9675385,0.000026591702,0.000059450136,0.00045907297,0.00032203668,0.0009697489,0.011498034,0.00016211037,0.000953231,0.017755626],"study_design_scores_gemma":[0.000004290328,0.000030832263,0.9975471,0.0000032003647,0.000008452803,0.00016549684,0.00015927792,0.0005053126,0.00039982973,0.0000256937,0.0011481633,0.0000024306446],"about_ca_topic_score_codex":0.0054879677,"about_ca_topic_score_gemma":0.010016147,"teacher_disagreement_score":0.0054879677,"about_ca_system_score_codex":0.00020069814,"about_ca_system_score_gemma":0.00017429421,"threshold_uncertainty_score":0.010912061},"labels":[],"label_agreement":null},{"id":"W2340721483","doi":"10.3847/0004-637x/818/2/142","title":"THE COMPACT STAR-FORMING COMPLEX AT THE HEART OF NGC 253*†‡","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Galaxy; Stars; Star formation; Spectral line; Population; Stellar population; Spectrograph; Stellar mass","score_opus":0.021666098456203143,"score_gpt":0.26520123473171076,"score_spread":0.2435351362755076,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2340721483","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99698347,0.00010578778,0.00016882621,0.000028364097,0.000004403534,0.0000013374166,0.000050198254,0.000010577481,0.0026469666],"genre_scores_gemma":[0.9994655,0.000031572872,0.0000766283,0.00000961704,0.0000066365646,4.5892713e-7,0.00007205128,0.0000030547376,0.00033438855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996483,0.0000021996043,0.0000012596703,0.000010234687,0.00000838477,0.000013031833],"domain_scores_gemma":[0.99986374,0.000010255498,0.000036640846,0.000010107697,0.000015850434,0.00006347693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000087368346,0.0001498074,0.00014124761,0.00033474067,0.00030643557,0.00048314346,0.00013440233,0.00010954118,0.0026639148],"category_scores_gemma":[0.00016188782,0.00004866453,0.000088324225,0.00018567595,0.00023315342,0.00023983225,0.00023617949,0.00014650726,0.00030639523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003976856,0.00009986088,0.69925356,0.000048910442,0.000058927086,0.0035005996,0.0013585918,0.0007652268,0.26645938,0.002686684,0.001521154,0.023849407],"study_design_scores_gemma":[0.0000049602136,0.000054233165,0.9905408,0.000006804163,0.000012869203,0.0011495602,0.00033129836,0.0006271781,0.0047393953,0.00027471728,0.0022530705,0.0000049457267],"about_ca_topic_score_codex":0.003378163,"about_ca_topic_score_gemma":0.003172309,"teacher_disagreement_score":0.003378163,"about_ca_system_score_codex":0.00025489656,"about_ca_system_score_gemma":0.000060935414,"threshold_uncertainty_score":0.008911669},"labels":[],"label_agreement":null},{"id":"W2341217455","doi":"10.3847/0004-637x/823/2/149","title":"SEARCHING FOR THE HR 8799 DEBRIS DISK WITH HST/STIS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Debris disk; Coronagraph; Telescope; Space Telescope Imaging Spectrograph; Planetesimal; Planet; Spitzer Space Telescope; Planetary system","score_opus":0.012481406648622014,"score_gpt":0.2343768443156279,"score_spread":0.2218954376670059,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2341217455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9816792,0.0001430749,0.010147619,0.00006133239,0.000016633112,0.000041233085,0.0025849433,0.00096335326,0.004362633],"genre_scores_gemma":[0.9725104,0.00003569142,0.021937938,0.00003405722,0.00001840532,0.000013453258,0.0048152506,0.000054111722,0.00058069325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968064,0.00002695694,0.000025864178,0.00007270978,0.00014232883,0.000051608098],"domain_scores_gemma":[0.99927217,0.00006148344,0.0002180501,0.00019396422,0.00017615194,0.00007815837],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005962305,0.00017067869,0.00016897211,0.001538566,0.00030142278,0.0006327001,0.00032459333,0.00022788746,0.0016076182],"category_scores_gemma":[0.0010519535,0.00013999123,0.00023154817,0.0009694189,0.00012877901,0.00028828907,0.00037253255,0.00015275915,0.0007565615],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021983986,0.00010415603,0.87147397,0.00005517481,0.00012880111,0.00034486395,0.00026369467,0.0032495449,0.04190505,0.00076921046,0.005296327,0.0761894],"study_design_scores_gemma":[0.000014160458,0.0000632496,0.95824206,0.000016030514,0.000037597936,0.00027753046,0.00012471921,0.02217682,0.013765942,0.000289836,0.00498158,0.000010496107],"about_ca_topic_score_codex":0.003904206,"about_ca_topic_score_gemma":0.006860236,"teacher_disagreement_score":0.003904206,"about_ca_system_score_codex":0.00030941438,"about_ca_system_score_gemma":0.00026146614,"threshold_uncertainty_score":0.007762909},"labels":[],"label_agreement":null},{"id":"W2341443050","doi":"10.3847/0004-637x/824/2/121","title":"SPECTROSCOPIC CHARACTERIZATION OF HD 95086 b WITH THE GEMINI PLANET IMAGER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of Victoria; Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Brown dwarf; Spectral energy distribution; Photometry (optics); Planet; Exoplanet; Spectral line; Surface gravity; Magnitude (astronomy); Stellar classification; Planetary mass; Effective temperature; Spectral resolution; Lambda; Astronomy; Stars; Galaxy","score_opus":0.005734480476292733,"score_gpt":0.19717305395360074,"score_spread":0.191438573477308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2341443050","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967349,0.0001217953,0.0003524686,0.000021389618,0.0000060342372,0.0000059049025,0.0013302248,0.0000368389,0.0013902924],"genre_scores_gemma":[0.99560237,0.000041048464,0.0009777837,0.000027296439,0.000007277645,0.0000063872853,0.0030038862,0.000007923198,0.00032609006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990857,0.000006601517,0.0000072636903,0.000033078803,0.000027122363,0.000017319717],"domain_scores_gemma":[0.99981564,0.000013040542,0.00005258698,0.000023557635,0.00004082002,0.000054487373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016103844,0.00016930401,0.00014550335,0.0009667068,0.00035771655,0.00028578812,0.00020348575,0.00015334408,0.0009246252],"category_scores_gemma":[0.00021727783,0.00009404782,0.0001253497,0.00053515605,0.000092546274,0.00016582108,0.00026275963,0.00016295815,0.00039378426],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003040617,0.00011931986,0.8683546,0.000057193978,0.00006170953,0.00037997912,0.00035857785,0.00040648045,0.107472,0.00021297898,0.0019325356,0.020340538],"study_design_scores_gemma":[0.000006084683,0.000039322193,0.9935807,0.0000048366082,0.000009727952,0.00029420183,0.00007251341,0.0005322843,0.003081905,0.000038890845,0.0023357028,0.0000038955045],"about_ca_topic_score_codex":0.0036622328,"about_ca_topic_score_gemma":0.006800336,"teacher_disagreement_score":0.0036622328,"about_ca_system_score_codex":0.00023466034,"about_ca_system_score_gemma":0.000048586902,"threshold_uncertainty_score":0.00728184},"labels":[],"label_agreement":null},{"id":"W2342202460","doi":"10.3847/0004-637x/824/2/86","title":"THE BOSS EMISSION-LINE LENS SURVEY. III. STRONG LENSING OF Lyα EMITTERS BY INDIVIDUAL GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Japan Society for the Promotion of Science; Chinese Academy of Sciences; U.S. Department of Energy; National Natural Science Foundation of China; York University; Carnegie Mellon University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; College of Engineering, Michigan State University; Johns Hopkins University; University of Utah; Ministry of Education, Culture, Sports, Science and Technology; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; National Aeronautics and Space Administration; Brookhaven National Laboratory","keywords":"Galaxy; Redshift; Gravitational lens; Lens (geology); Boss; Quasar; Sky; Dark matter; Baryon","score_opus":0.016025192867725264,"score_gpt":0.23249052172557283,"score_spread":0.21646532885784756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2342202460","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97420734,0.000654432,0.00055414106,0.00018896289,0.0000092147675,0.000036346013,0.018790642,0.0001326273,0.005426353],"genre_scores_gemma":[0.9696182,0.00033156332,0.0012261744,0.0000994764,0.00004182985,0.000026675152,0.026121885,0.000040972664,0.0024933303],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966526,0.000041938,0.00002235887,0.000060838604,0.00010757065,0.00010197774],"domain_scores_gemma":[0.9993222,0.00002847421,0.0002925368,0.00005319429,0.00009431247,0.00020928087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006670795,0.00028194563,0.00022700115,0.0025313075,0.00033478186,0.0005375138,0.00020797094,0.00012504552,0.0025338312],"category_scores_gemma":[0.00047108188,0.0001952479,0.00022391132,0.0015143717,0.00024018009,0.00031370856,0.00086045376,0.00015352463,0.0007938233],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011373467,0.000015767222,0.9771518,0.00003443379,0.000058255868,0.00006197994,0.00010858063,0.00012500296,0.0055017723,0.0003585759,0.0047709118,0.011699213],"study_design_scores_gemma":[0.00000732409,0.000011266749,0.9964636,0.0000049066493,0.000009006285,0.000032902048,0.000050054412,0.00017437615,0.0005538937,0.000030093674,0.0026602962,0.0000024397445],"about_ca_topic_score_codex":0.026844544,"about_ca_topic_score_gemma":0.08735343,"teacher_disagreement_score":0.026844544,"about_ca_system_score_codex":0.00066750875,"about_ca_system_score_gemma":0.00035390255,"threshold_uncertainty_score":0.053376555},"labels":[],"label_agreement":null},{"id":"W2342649757","doi":"10.3847/0004-637x/824/2/111","title":"INTERPRETING THE SUBTLE SPECTRAL VARIATIONS OF THE 11.2 AND 12.7 μm POLYCYCLIC AROMATIC HYDROCARBON BANDS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Reflection nebula; Polycyclic aromatic hydrocarbon; Emission spectrum; Spectral bands; Reflection (computer programming); Spectral line; Cationic polymerization; Hydrocarbon","score_opus":0.005919631852335661,"score_gpt":0.2108707328980759,"score_spread":0.20495110104574024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2342649757","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99410605,0.00009799078,0.003894683,0.000019703231,0.000003029087,0.0000047551266,0.00029105318,0.00006212299,0.0015206076],"genre_scores_gemma":[0.9975802,0.000030946052,0.0018451764,0.00000867362,0.000003983669,0.0000027883232,0.00025080543,0.000011476617,0.0002659825],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999503,0.000004163706,0.0000015098939,0.000014024593,0.000013505352,0.000016466143],"domain_scores_gemma":[0.9998684,0.000024226043,0.00004025296,0.0000150382475,0.000027871987,0.00002412966],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014139693,0.00017516255,0.00009797618,0.00079552864,0.00017048448,0.0002603125,0.00015654736,0.00013826304,0.001082541],"category_scores_gemma":[0.00021006969,0.000095525524,0.00015437619,0.00043314107,0.00018174117,0.00019447591,0.00028254866,0.000142388,0.00025571906],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017286281,0.00004214683,0.63478774,0.000060685186,0.00006437862,0.00020404127,0.00043216572,0.0021471782,0.3243416,0.0006623969,0.00039342942,0.036691394],"study_design_scores_gemma":[0.0000023533362,0.000018455165,0.98646563,0.0000030836968,0.000019182467,0.00014428084,0.00009888352,0.0024639857,0.009482653,0.00022600476,0.001069756,0.0000056716453],"about_ca_topic_score_codex":0.0016296253,"about_ca_topic_score_gemma":0.0039009044,"teacher_disagreement_score":0.0016296253,"about_ca_system_score_codex":0.00009756168,"about_ca_system_score_gemma":0.00007712757,"threshold_uncertainty_score":0.003621459},"labels":[],"label_agreement":null},{"id":"W2342785008","doi":"10.3847/0004-637x/831/1/98","title":"GENERAL-RELATIVISTIC THREE-DIMENSIONAL MULTI-GROUP NEUTRINO RADIATION-HYDRODYNAMICS SIMULATIONS OF CORE-COLLAPSE SUPERNOVAE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Octant (instrument); Neutrino; Supernova; Circular symmetry; Asymmetry; Core (optical fiber); Symmetry (geometry); Rotational symmetry","score_opus":0.022350490091708246,"score_gpt":0.2844338624339715,"score_spread":0.26208337234226325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2342785008","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995323,0.000050841594,0.0018292835,0.00009842337,0.000016907976,0.000021152253,0.00019111829,0.00009525456,0.0023739855],"genre_scores_gemma":[0.9962286,0.000037133577,0.0028358924,0.00006176298,0.0000099171,0.000028946368,0.00030723066,0.00004063255,0.00044987115],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997938,0.000068167516,0.0000094854695,0.000019893047,0.000044192017,0.00006433446],"domain_scores_gemma":[0.9989832,0.00044111826,0.0001161084,0.00009771267,0.00013727257,0.00022452738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063264015,0.00049811526,0.00083498925,0.00048009492,0.0006431347,0.0007100276,0.0016115698,0.0011172822,0.0013966371],"category_scores_gemma":[0.002181241,0.00039892303,0.0010310226,0.0005860293,0.0011883683,0.00038901748,0.0009172768,0.0010361751,0.0001304297],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019740517,0.0002002679,0.0050733294,0.000024915744,0.00007798569,0.00015898024,0.00009771044,0.98967135,0.00167722,0.001498659,0.00022616991,0.0010959839],"study_design_scores_gemma":[0.00006477268,0.00006662134,0.0021951238,0.0000038103158,0.0000105914605,0.000017485112,0.000041451505,0.99657553,0.00049983617,0.00037733786,0.00013694407,0.0000104177225],"about_ca_topic_score_codex":0.020875389,"about_ca_topic_score_gemma":0.0121574905,"teacher_disagreement_score":0.020875389,"about_ca_system_score_codex":0.0011569561,"about_ca_system_score_gemma":0.0010079963,"threshold_uncertainty_score":0.04150778},"labels":[],"label_agreement":null},{"id":"W2342809927","doi":"10.3847/0004-637x/824/1/10","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY (NGVS). XIII. THE LUMINOSITY AND MASS FUNCTION OF GALAXIES IN THE CORE OF THE VIRGO CLUSTER AND THE CONTRIBUTION FROM DISRUPTED SATELLITES*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Queen's University; University of Waterloo; Herzberg Institute of Astrophysics","funders":"Centre National de la Recherche Scientifique; Agence Nationale de la Recherche","keywords":"Virgo Cluster; Globular cluster; Luminosity function; Galaxy; Luminosity; Dwarf galaxy; Galaxy cluster; Cluster (spacecraft)","score_opus":0.015959389379455926,"score_gpt":0.2126281117540941,"score_spread":0.19666872237463817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2342809927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.973825,0.00039865935,0.0007242899,0.00008362891,0.000015745465,0.000028613118,0.020571556,0.00009580415,0.0042567444],"genre_scores_gemma":[0.95728457,0.00015316147,0.0015961595,0.00006615705,0.000019058027,0.000034030254,0.039498664,0.000026522914,0.0013216616],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976844,0.00004347003,0.000010407526,0.00005393417,0.000074591386,0.000049248225],"domain_scores_gemma":[0.99943596,0.000073024254,0.0001611686,0.000095137366,0.00010346682,0.00013124086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044668865,0.00019944937,0.00019258782,0.0014211155,0.00018740924,0.0003692723,0.00035276316,0.00020220538,0.0010870156],"category_scores_gemma":[0.0009337812,0.0001098421,0.00023167141,0.0012870266,0.00016818433,0.00021971672,0.0006163583,0.00022130327,0.00049245404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000074013755,0.000020905129,0.9855209,0.000028619139,0.00007521359,0.00003226106,0.0001161462,0.00041831398,0.0015941762,0.00025376186,0.004071339,0.007794193],"study_design_scores_gemma":[0.0000023825994,0.0000066894595,0.9977963,0.0000038804633,0.000007804104,0.000020225112,0.000020079167,0.000323154,0.00021010372,0.000034093133,0.0015732531,0.000002018383],"about_ca_topic_score_codex":0.03773628,"about_ca_topic_score_gemma":0.054758556,"teacher_disagreement_score":0.03773628,"about_ca_system_score_codex":0.0006374284,"about_ca_system_score_gemma":0.00027536968,"threshold_uncertainty_score":0.07503331},"labels":[],"label_agreement":null},{"id":"W2342845990","doi":"10.3847/0004-637x/822/1/17","title":"GAS PHASE ABSORPTION SPECTROSCOPY OF AND IN A CRYOGENIC ION TRAP: COMPARISON WITH ASTRONOMICAL MEASUREMENTS*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Fullerene Chemistry and Applications","field":"Chemistry","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Absorption spectroscopy; Absorption (acoustics); Atomic physics; Astrophysics; Analytical Chemistry (journal); Optics; Chemistry","score_opus":0.024569268982022965,"score_gpt":0.27452273128177485,"score_spread":0.24995346229975188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2342845990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98893785,0.0012398387,0.004917852,0.00012419978,0.00003981208,0.000022148492,0.00077832496,0.00012486758,0.0038152223],"genre_scores_gemma":[0.9936406,0.0003928781,0.0043990547,0.00005577704,0.00002932001,0.000015920928,0.0004804938,0.000020597081,0.00096524437],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998122,0.00002024102,0.0000047034923,0.00006334534,0.00006967163,0.000029910121],"domain_scores_gemma":[0.99982136,0.000041384228,0.00004647038,0.000023531587,0.000046916794,0.000020358522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000339725,0.00020002206,0.00013554921,0.00040716515,0.00043969412,0.00037224483,0.00048993673,0.00035066684,0.0021502115],"category_scores_gemma":[0.0003873016,0.00010612889,0.000098117926,0.00038406282,0.00041471838,0.0003980677,0.00039643855,0.000293405,0.000396064],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002788563,0.000047751248,0.008161851,0.00008617278,0.00002663347,0.000094973024,0.00017692488,0.0002465347,0.98569196,0.0004818191,0.00039808822,0.004308416],"study_design_scores_gemma":[0.00007336225,0.0006220823,0.07449725,0.000027033495,0.0000631234,0.0008083471,0.00044289624,0.0062279827,0.90482736,0.0005013176,0.01187338,0.00003588861],"about_ca_topic_score_codex":0.0011235104,"about_ca_topic_score_gemma":0.0015510019,"teacher_disagreement_score":0.0021502115,"about_ca_system_score_codex":0.00022575339,"about_ca_system_score_gemma":0.00016675514,"threshold_uncertainty_score":0.007193148},"labels":[],"label_agreement":null},{"id":"W2343467587","doi":"10.3847/0004-637x/824/1/30","title":"CHANG-ES. VII. MAGNETIC OUTFLOWS FROM THE VIRGO CLUSTER GALAXY NGC 4388","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Queen's University","funders":"","keywords":"Physics; Astrophysics; Virgo Cluster; Halo; Intracluster medium; Galaxy; Ram pressure; Galaxy cluster; Outflow; Astronomy; Radio galaxy; Radio halo; Star formation","score_opus":0.006889723451369639,"score_gpt":0.19587072091599997,"score_spread":0.18898099746463032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2343467587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994691,0.000018051991,0.000043647076,0.000007879663,3.1175995e-7,6.7560535e-7,0.000039216546,0.0000072086837,0.00041387876],"genre_scores_gemma":[0.99964714,0.000010631403,0.000085522275,0.0000051184675,8.942968e-7,6.82269e-7,0.000120518125,0.0000023555178,0.00012704813],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997365,0.000004042842,7.445636e-7,0.0000051590173,0.0000063729854,0.000010063223],"domain_scores_gemma":[0.9999279,0.000010826462,0.000021046591,0.0000086455475,0.0000084309495,0.000023058885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000068867215,0.00012318014,0.00012264463,0.00024174507,0.00017472485,0.00018493245,0.00007557995,0.000112209265,0.00059797306],"category_scores_gemma":[0.00012428887,0.00005668422,0.0000711368,0.00016733189,0.00008211524,0.00006206494,0.00022885771,0.00010154971,0.00011217664],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055838545,0.00010791759,0.7118295,0.000048665377,0.000060556955,0.0015643172,0.0006202608,0.005327671,0.25886908,0.00079788914,0.0006055072,0.019610208],"study_design_scores_gemma":[0.000010850477,0.00003749197,0.9927704,0.0000024065478,0.000008258552,0.0001864726,0.000085526655,0.002663647,0.003457404,0.000112448615,0.00066131866,0.0000038387925],"about_ca_topic_score_codex":0.0043231877,"about_ca_topic_score_gemma":0.004829729,"teacher_disagreement_score":0.0043231877,"about_ca_system_score_codex":0.00017144775,"about_ca_system_score_gemma":0.000064387175,"threshold_uncertainty_score":0.008596063},"labels":[],"label_agreement":null},{"id":"W2343543883","doi":"10.3847/0004-637x/825/1/74","title":"BROADBAND OBSERVATIONS OF HIGH REDSHIFT BLAZARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; York University; Carnegie Mellon University; University of Arizona; Office of Science; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; College of Engineering, Michigan State University; Goddard Space Flight Center; Harvard University; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Blazar; Astrophysics; Redshift; Luminosity; Fermi Gamma-ray Space Telescope; Quasar; Astronomy; Galaxy; Gamma ray","score_opus":0.013309303543035677,"score_gpt":0.21716368359094695,"score_spread":0.2038543800479113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2343543883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983126,0.00008068897,0.00022678133,0.000013723216,0.0000018184425,0.0000041434378,0.0004798155,0.000043892265,0.0008365745],"genre_scores_gemma":[0.9985078,0.000036999012,0.00042190278,0.000010719929,0.0000059195986,0.0000025262686,0.0008219569,0.0000061883406,0.00018594843],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998161,0.000019066394,0.0000092074015,0.000055754055,0.000045968965,0.000053916636],"domain_scores_gemma":[0.9994579,0.000072023395,0.00023543759,0.000038287908,0.00004492364,0.00015148288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022020203,0.00023163031,0.00019984037,0.001770368,0.00029793687,0.00048779623,0.00015204579,0.00023214525,0.0010565721],"category_scores_gemma":[0.00043231485,0.00017318262,0.00019331378,0.00096173736,0.00019651027,0.00021298054,0.00030037886,0.00020604553,0.00025823628],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020059732,0.0000848297,0.91617185,0.000031793817,0.00011873579,0.00023721118,0.00032237187,0.00070749316,0.07027736,0.000291254,0.00063802797,0.010918449],"study_design_scores_gemma":[0.0000035629505,0.000022915468,0.99878615,0.0000017872738,0.00000882139,0.00007638876,0.00003512548,0.00021150308,0.00051375304,0.000018414521,0.0003190055,0.0000025563309],"about_ca_topic_score_codex":0.004744945,"about_ca_topic_score_gemma":0.010228153,"teacher_disagreement_score":0.004744945,"about_ca_system_score_codex":0.00029732764,"about_ca_system_score_gemma":0.0000969032,"threshold_uncertainty_score":0.00943464},"labels":[],"label_agreement":null},{"id":"W2344201901","doi":"10.3847/0004-637x/824/2/130","title":"C IV BROAD ABSORPTION LINE ACCELERATION IN SLOAN DIGITAL SKY SURVEY QUASARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Acceleration; Galaxy; Sky; Line (geometry); Spectral line; Black hole (networking); Magnitude (astronomy)","score_opus":0.015007381357423513,"score_gpt":0.232312264333999,"score_spread":0.2173048829765755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2344201901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99827254,0.00008716665,0.00012841586,0.000010710169,0.0000014283548,0.0000043795612,0.00090368994,0.000015670385,0.0005759581],"genre_scores_gemma":[0.99803525,0.00005542947,0.00016799214,0.0000098928795,0.0000032726148,0.0000045402444,0.001568968,0.0000045296965,0.00015019247],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996946,0.0000477949,0.000021417318,0.00007173934,0.00008443517,0.000079970436],"domain_scores_gemma":[0.9976031,0.00031623463,0.0010806882,0.00023741211,0.0004071165,0.00035557654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007234659,0.0002638821,0.00015956952,0.0027425392,0.00033487187,0.0006192387,0.00017619206,0.00013497785,0.00069366756],"category_scores_gemma":[0.0012453556,0.00010808769,0.00024654364,0.0018938133,0.00031300468,0.0002404468,0.0006511543,0.00016078558,0.00022269455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000020740037,0.0000102079075,0.99666095,0.0000071806053,0.00002150726,0.000023401879,0.00006436257,0.00006430864,0.0008335727,0.00002058739,0.0001146244,0.0021584034],"study_design_scores_gemma":[5.4722e-7,0.000007979172,0.999634,0.0000012695829,0.0000050339795,0.0000187643,0.0000359484,0.000052314088,0.00009701709,0.000006598628,0.00013945265,9.800505e-7],"about_ca_topic_score_codex":0.018492328,"about_ca_topic_score_gemma":0.029475065,"teacher_disagreement_score":0.018492328,"about_ca_system_score_codex":0.0004352207,"about_ca_system_score_gemma":0.00026472678,"threshold_uncertainty_score":0.03676939},"labels":[],"label_agreement":null},{"id":"W2345263333","doi":"10.3847/1538-4357/835/2/128","title":"The Impact of Modeling Assumptions in Galactic Chemical Evolution Models","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Galaxy; Supernova; Astrophysics; Degeneracy (biology); Physics; Galaxy formation and evolution; Chemical evolution; Star formation; Statistical physics","score_opus":0.018225586431613434,"score_gpt":0.26599442787716576,"score_spread":0.24776884144555233,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2345263333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9627609,0.000109980196,0.030543197,0.0005365758,0.000028608081,0.00004794019,0.00051103,0.000335818,0.0051260297],"genre_scores_gemma":[0.9917848,0.00005330414,0.0075309663,0.00008225892,0.0000051093243,0.00003324623,0.00021553144,0.00007853118,0.00021621845],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99736434,0.0014828808,0.00018248156,0.000274353,0.0004762841,0.00021964383],"domain_scores_gemma":[0.972843,0.021581605,0.0016579615,0.0023107443,0.0012410679,0.00036573116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0055297497,0.0007256399,0.0006850009,0.00062789617,0.0008777986,0.0022483692,0.0019588964,0.0010843301,0.001129797],"category_scores_gemma":[0.03374571,0.00055272435,0.0007955339,0.00075875537,0.0011039653,0.0016897493,0.001288855,0.0012920832,0.000178966],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012011565,0.000049512513,0.015145138,0.000029082572,0.000043762662,0.000059044643,0.00008291873,0.9771614,0.0006486969,0.004571373,0.00014499827,0.0019439224],"study_design_scores_gemma":[0.000020736341,0.000040366205,0.0011895178,0.000016586762,0.000021051805,0.000016369446,0.000047091093,0.99611086,0.0009272512,0.0013875832,0.00021066034,0.000011902644],"about_ca_topic_score_codex":0.023383759,"about_ca_topic_score_gemma":0.01048495,"teacher_disagreement_score":0.023383759,"about_ca_system_score_codex":0.0019043556,"about_ca_system_score_gemma":0.0014247017,"threshold_uncertainty_score":0.04649532},"labels":[],"label_agreement":null},{"id":"W2346014611","doi":"10.3847/0004-637x/826/1/34","title":"EXPANDING MOLECULAR BUBBLE SURROUNDING TYCHO’S SUPERNOVA REMNANT (SN 1572) OBSERVED WITH THE IRAM 30 m TELESCOPE: EVIDENCE FOR A SINGLE-DEGENERATE PROGENITOR","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Supernova remnant; Bubble; Line (geometry); Supernova; Outflow; White dwarf; Shock wave","score_opus":0.05610071318931798,"score_gpt":0.27437960849462056,"score_spread":0.2182788953053026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2346014611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992207,0.000063698964,0.00012486921,0.000011294929,0.0000020097164,0.0000039480606,0.000056875368,0.000011675906,0.0005048178],"genre_scores_gemma":[0.999509,0.000020203452,0.00023364497,0.000009083355,0.0000033148476,0.0000029557584,0.000111593894,0.0000025218678,0.00010765441],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999609,0.0000021974213,0.0000022889458,0.000011819662,0.000010400142,0.000012405236],"domain_scores_gemma":[0.9998012,0.000016241711,0.00007330196,0.000016514732,0.000021330217,0.00007140576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001334396,0.00015092964,0.00021917064,0.00044803278,0.00029267304,0.00030667725,0.00025374623,0.0002852801,0.0011056345],"category_scores_gemma":[0.00022924121,0.00017996175,0.00016439475,0.00022594375,0.00025655548,0.00019385573,0.00049315044,0.00024299018,0.00022973704],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022518316,0.00006595638,0.7542247,0.000047628404,0.00006377051,0.006200932,0.0004307558,0.00026700113,0.2353707,0.00027180908,0.00023009363,0.0026014892],"study_design_scores_gemma":[0.000010880871,0.000093609204,0.98785186,0.000007764254,0.000022841663,0.003654121,0.00032451501,0.001148769,0.006123658,0.000055231907,0.0006998267,0.0000068596455],"about_ca_topic_score_codex":0.0040237736,"about_ca_topic_score_gemma":0.0043413737,"teacher_disagreement_score":0.0040237736,"about_ca_system_score_codex":0.00019799345,"about_ca_system_score_gemma":0.00013010562,"threshold_uncertainty_score":0.008000672},"labels":[],"label_agreement":null},{"id":"W2346599256","doi":"10.3847/0004-637x/825/1/10","title":"THE FIRST LOW-MASS BLACK HOLE X-RAY BINARY IDENTIFIED IN QUIESCENCE OUTSIDE OF A GLOBULAR CLUSTER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; University of Alberta","funders":"Australian Research Council; Natural Sciences and Engineering Research Council of Canada; Associated Universities; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Space Telescope Science Institute; Vetenskapsrådet; National Science Foundation","keywords":"Physics; Astrophysics; Globular cluster; Astronomy; Neutron star; Galaxy; Population; Black hole (networking); Luminosity; Star cluster","score_opus":0.008884283510631946,"score_gpt":0.22189476635828717,"score_spread":0.21301048284765522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2346599256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99922824,0.00004351247,0.000045521036,0.00002092533,0.0000043267974,0.0000039530373,0.000033640255,0.000005729507,0.0006142243],"genre_scores_gemma":[0.99956006,0.000013051789,0.000056564826,0.000028621434,0.00000757499,0.000001135128,0.000076402175,0.0000017068428,0.00025473663],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999002,0.0000056379304,0.000007389296,0.000027212012,0.000023082492,0.00003642867],"domain_scores_gemma":[0.9997224,0.000019319417,0.000042188352,0.000024911124,0.000034193006,0.00015699455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012740323,0.00018154408,0.00021309043,0.0005969367,0.00097238313,0.000613893,0.00033685035,0.0003634,0.0014421028],"category_scores_gemma":[0.00034473714,0.000119266944,0.000108376255,0.0003099201,0.00043296546,0.00022670807,0.0007372828,0.00029696955,0.0003663768],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020865699,0.00012846332,0.9645604,0.000022031036,0.000021528283,0.010666455,0.0013700434,0.00007249109,0.014838899,0.0003286466,0.0004500381,0.007332419],"study_design_scores_gemma":[0.000009456993,0.00021492082,0.99168736,0.000006475925,0.0000142086965,0.0050069713,0.00063121406,0.0002447533,0.00081654167,0.00010933931,0.001253656,0.0000051377224],"about_ca_topic_score_codex":0.00860564,"about_ca_topic_score_gemma":0.011897778,"teacher_disagreement_score":0.00860564,"about_ca_system_score_codex":0.00043928061,"about_ca_system_score_gemma":0.00025241115,"threshold_uncertainty_score":0.017111063},"labels":[],"label_agreement":null},{"id":"W2346987996","doi":"10.3847/0004-637x/826/2/114","title":"A SYSTEMATIC SURVEY OF PROTOCLUSTERS AT z ∼ 3–6 IN THE CFHTLS DEEP FIELDS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Galaxy; Halo; Sky; Luminosity; Telescope; Galaxy cluster; Cluster (spacecraft); Redshift","score_opus":0.010813152170803933,"score_gpt":0.2227935261197321,"score_spread":0.21198037394892816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2346987996","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991949,0.00004682948,0.000086206805,0.000014558544,8.934602e-7,0.000005804729,0.00028230806,0.000007139809,0.00036128485],"genre_scores_gemma":[0.9988167,0.00003477544,0.0001941154,0.000023911547,0.0000038599223,0.0000048081697,0.0006368676,0.000002125799,0.00028296412],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997665,0.000011991389,0.00000897284,0.000048394802,0.00006788838,0.00009620657],"domain_scores_gemma":[0.9989398,0.00010173235,0.0003431153,0.000083163395,0.00017928585,0.00035289963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028867,0.00017598135,0.00015401846,0.0025718783,0.0006983135,0.00040839237,0.00026697377,0.0001666887,0.00096422835],"category_scores_gemma":[0.0005085897,0.00011114066,0.00015399452,0.0008664098,0.0004212921,0.0002781577,0.0006402523,0.00018486245,0.00018142778],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004381451,0.00001652947,0.9871777,0.0000061635315,0.000009626239,0.00014249465,0.00028870403,0.000036492354,0.0077530397,0.00007135303,0.0002041907,0.004249918],"study_design_scores_gemma":[0.0000013258192,0.000017219165,0.9988979,0.0000024118992,0.000003808578,0.000091053684,0.000113882365,0.000058770966,0.00044575715,0.000016242038,0.0003496578,0.0000019473473],"about_ca_topic_score_codex":0.026647493,"about_ca_topic_score_gemma":0.04811463,"teacher_disagreement_score":0.026647493,"about_ca_system_score_codex":0.0006689267,"about_ca_system_score_gemma":0.0004224104,"threshold_uncertainty_score":0.052984834},"labels":[],"label_agreement":null},{"id":"W2347958330","doi":"10.3847/0004-637x/822/2/86","title":"FALSE POSITIVE PROBABILITIES FOR ALL KEPLER OBJECTS OF INTEREST: 1284 NEWLY VALIDATED PLANETS AND 428 LIKELY FALSE POSITIVES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":427,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"False positive paradox; Planet; Exoplanet; Kepler; Transit (satellite); False positive rate; False alarm","score_opus":0.023884785700974288,"score_gpt":0.2471470792306161,"score_spread":0.2232622935296418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2347958330","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8871164,0.0010594885,0.0966159,0.00035883844,0.00012849874,0.00012060165,0.00474577,0.0030712506,0.006783275],"genre_scores_gemma":[0.97285324,0.00013279443,0.021556161,0.00007451977,0.000035001172,0.000043617732,0.0038675473,0.0002747217,0.0011622509],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99729556,0.0005285479,0.00021972462,0.00082183315,0.00084000675,0.00029428044],"domain_scores_gemma":[0.9834509,0.011621199,0.0013914724,0.0017424793,0.0014493737,0.00034451805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004909385,0.00069864176,0.0005457139,0.0022722052,0.0009492488,0.0020244487,0.0008133046,0.00082570635,0.0046386747],"category_scores_gemma":[0.027198697,0.00035107596,0.0010940603,0.00093905325,0.000691909,0.0013571215,0.0015086303,0.0008244193,0.0014210605],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012807449,0.00013925748,0.78782535,0.00045316803,0.00049247977,0.0020502943,0.00065439416,0.054750655,0.014726432,0.0073306463,0.010087894,0.120208666],"study_design_scores_gemma":[0.00014263167,0.00038864225,0.37569413,0.00029758646,0.0006552715,0.010215712,0.0006612295,0.46872038,0.09382809,0.01896601,0.030185632,0.00024475995],"about_ca_topic_score_codex":0.0022496714,"about_ca_topic_score_gemma":0.0020696712,"teacher_disagreement_score":0.004909385,"about_ca_system_score_codex":0.0005882308,"about_ca_system_score_gemma":0.00048171953,"threshold_uncertainty_score":0.025963604},"labels":[],"label_agreement":null},{"id":"W2353371772","doi":"10.3847/0004-637x/826/2/147","title":"THE PECULIAR DEBRIS DISK OF HD 111520 AS RESOLVED BY THE GEMINI PLANET IMAGER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Université de Montréal; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Debris disk; Brightness; Asymmetry; Astrophysics; Planet; Polarization (electrochemistry); Stars; Debris; Position angle; Surface brightness; Astronomy; Planetary system","score_opus":0.006562191257750909,"score_gpt":0.2142779344434427,"score_spread":0.2077157431856918,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2353371772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991534,0.00003288877,0.00009493321,0.000010584279,0.0000017191052,0.0000017835899,0.00016660042,0.000008395594,0.00052982505],"genre_scores_gemma":[0.9992643,0.000009934294,0.0002030898,0.000009012025,0.0000018549503,0.0000012384546,0.0003500208,0.0000023482896,0.00015817689],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994314,0.000006021858,0.000002962179,0.00002008527,0.000010153803,0.000017612645],"domain_scores_gemma":[0.9998952,0.000011890812,0.000027145239,0.000016313423,0.000015745767,0.000033674332],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012914842,0.00014957346,0.00014916896,0.00030964368,0.00032065331,0.00037687153,0.00011965207,0.00018344948,0.0010138323],"category_scores_gemma":[0.00020991612,0.00014061118,0.00007567833,0.00025545637,0.00016581539,0.00016996493,0.00025392507,0.00014128884,0.00024053825],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046744494,0.00008266528,0.71896374,0.00004946084,0.00006785764,0.0008770606,0.0005907407,0.00091606413,0.26617238,0.00025912648,0.00081908196,0.010734268],"study_design_scores_gemma":[0.000004776194,0.000027099682,0.99649847,0.0000024344076,0.000008236838,0.0002100593,0.000073516,0.0004962799,0.0022282738,0.000011857494,0.00043637725,0.0000027113551],"about_ca_topic_score_codex":0.0048155147,"about_ca_topic_score_gemma":0.00998926,"teacher_disagreement_score":0.0048155147,"about_ca_system_score_codex":0.0002849319,"about_ca_system_score_gemma":0.00007122558,"threshold_uncertainty_score":0.00957495},"labels":[],"label_agreement":null},{"id":"W2357848260","doi":"10.3847/0004-637x/826/1/71","title":"APERTURE EFFECTS ON THE OXYGEN ABUNDANCE DETERMINATIONS FROM CALIFA DATA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"FP7 People: Marie-Curie Actions; Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Fundação para a Ciência e a Tecnologia; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Harvard University; Instituto de Astrofísica de Andalucía; Max-Planck-Gesellschaft; Ministerio de Economía y Competitividad; York University; Instituto de Astrofísica de Canarias; Carnegie Mellon University; University of Arizona; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ohio State University; Junta de Andalucía; New Mexico State University; Yale University; Vanderbilt University; National Science Foundation; U.S. Department of Energy; California Institute of Technology; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration","keywords":"Abundance (ecology); Environmental science; Oxygen; Aperture (computer memory); Ecology; Chemistry; Physics; Biology","score_opus":0.016602481167966365,"score_gpt":0.24108392605518855,"score_spread":0.2244814448872222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2357848260","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9893758,0.00024993691,0.002172048,0.000043858374,0.000014078923,0.000011135286,0.0051522907,0.00055739016,0.0024234725],"genre_scores_gemma":[0.9829549,0.00007126169,0.004418425,0.000029412666,0.000010901229,0.000016127835,0.011724543,0.00017959921,0.0005947591],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99921024,0.00008399688,0.000042617674,0.00029350552,0.0002897623,0.000079788435],"domain_scores_gemma":[0.99700373,0.0010513323,0.00044353778,0.0007388952,0.0006262334,0.00013625265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009901342,0.0003494834,0.00032444514,0.0007917345,0.00027897864,0.00076828565,0.00044940325,0.0002731901,0.0010508632],"category_scores_gemma":[0.004633719,0.00027269305,0.0003709449,0.0009821446,0.00021239753,0.0003774288,0.00049203227,0.0002632328,0.00042715963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050279265,0.00007195241,0.876476,0.00014040012,0.0001756552,0.0001566529,0.00021288058,0.054959442,0.023035793,0.00054246606,0.003749765,0.039976332],"study_design_scores_gemma":[0.00003530846,0.00005009971,0.911804,0.000035440706,0.000046587753,0.000101510814,0.00012860088,0.075766616,0.0072952206,0.00019969963,0.0045110537,0.000025809568],"about_ca_topic_score_codex":0.02887181,"about_ca_topic_score_gemma":0.040275242,"teacher_disagreement_score":0.02887181,"about_ca_system_score_codex":0.00071892736,"about_ca_system_score_gemma":0.00032133516,"threshold_uncertainty_score":0.0574075},"labels":[],"label_agreement":null},{"id":"W2358512287","doi":"10.3847/0004-637x/827/1/29","title":"RE-EVALUATION OF THE<sup>16</sup>O(<i>N</i>,<i>γ</i>)<sup>17</sup>O CROSS SECTION AT ASTROPHYSICAL ENERGIES AND ITS ROLE AS A NEUTRON POISON IN THE<i>s</i>-PROCESS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; TRIUMF","funders":"","keywords":"s-process; Neutron; Helium; Cross section (physics); Nuclear astrophysics; Nucleosynthesis; Neutron star; Stars; Neutron capture","score_opus":0.016178903007117915,"score_gpt":0.29923240132222184,"score_spread":0.2830534983151039,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2358512287","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5246749,0.07861527,0.26463094,0.012161176,0.0045568235,0.0003718634,0.015203943,0.0041794875,0.09560561],"genre_scores_gemma":[0.8743973,0.020879798,0.07969508,0.0027510782,0.0006595139,0.00022089457,0.006594508,0.001251947,0.0135499295],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99678826,0.00069109694,0.00021958143,0.00079414464,0.0013395423,0.00016737278],"domain_scores_gemma":[0.9835669,0.0052316305,0.0020369443,0.0035770272,0.005218714,0.00036877193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005577978,0.0013885306,0.0006104382,0.0018729746,0.0006218131,0.0012121426,0.0029830176,0.0016853879,0.004291334],"category_scores_gemma":[0.009837275,0.00048116993,0.0008015862,0.0010302131,0.0009282752,0.003136945,0.0012719126,0.0018732152,0.0025606381],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0036677131,0.00065140484,0.14214379,0.0052687842,0.0008595203,0.0006026711,0.0012607062,0.028352546,0.2892353,0.03144045,0.03854544,0.45797175],"study_design_scores_gemma":[0.00009518797,0.0015487393,0.13338166,0.0010892923,0.0009604229,0.0017008404,0.00089537905,0.02507553,0.5774688,0.018781286,0.23866214,0.00034067017],"about_ca_topic_score_codex":0.003869391,"about_ca_topic_score_gemma":0.0074913655,"teacher_disagreement_score":0.005577978,"about_ca_system_score_codex":0.0014360845,"about_ca_system_score_gemma":0.00077880814,"threshold_uncertainty_score":0.02949953},"labels":[],"label_agreement":null},{"id":"W2359598440","doi":"10.3847/0004-637x/831/2/159","title":"A UNIFIED MODEL OF GRAIN ALIGNMENT: RADIATIVE ALIGNMENT OF INTERSTELLAR GRAINS WITH MAGNETIC INCLUSIONS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":152,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Radiative transfer; Magnetic field; Paramagnetism; Accretion (finance); Anisotropy; Attractor; Astrophysics; Computational physics; Condensed matter physics; Optics; Quantum mechanics","score_opus":0.010924363825590717,"score_gpt":0.22283438331363847,"score_spread":0.21191001948804775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2359598440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.69046265,0.0008488142,0.25552666,0.0012519084,0.00016201308,0.00011961337,0.0002066781,0.00051390176,0.05090779],"genre_scores_gemma":[0.99254215,0.00013902881,0.0032318018,0.000051957217,0.00003455978,0.000046730176,0.00002954476,0.000034673674,0.00388957],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998734,0.000023267743,0.000004770351,0.000030349405,0.00002736819,0.00004075096],"domain_scores_gemma":[0.9998066,0.000031813484,0.000059351245,0.000025160994,0.000030801915,0.000046330744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023769736,0.00037162576,0.0005718177,0.00041676278,0.00070610206,0.00096194627,0.0011940997,0.0010622339,0.0029520697],"category_scores_gemma":[0.0005895119,0.00029759307,0.000505511,0.00030482712,0.0011906141,0.0012691794,0.00066511414,0.00043117767,0.0004428242],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000734713,0.00009157282,0.0016550644,0.000058726335,0.000025495681,0.000441469,0.00017414895,0.7565708,0.028921241,0.20787539,0.0009114099,0.0032012148],"study_design_scores_gemma":[0.00003176103,0.000032316006,0.0007645172,0.0000039946913,0.0000058869045,0.000042787215,0.00003786004,0.98045415,0.0008572714,0.017238349,0.00051853375,0.000012582093],"about_ca_topic_score_codex":0.004326865,"about_ca_topic_score_gemma":0.0016239586,"teacher_disagreement_score":0.004326865,"about_ca_system_score_codex":0.0011903136,"about_ca_system_score_gemma":0.00044867944,"threshold_uncertainty_score":0.009875655},"labels":[],"label_agreement":null},{"id":"W2366293464","doi":"10.3847/0004-637x/822/2/115","title":"DETECTION OF HF TOWARD PKS 1830–211, SEARCH FOR INTERSTELLAR H<sub>2</sub>F<sup>+</sup>, AND LABORATORY STUDY OF H<sub>2</sub>F<sup>+</sup> AND H<sub>2</sub>Cl<sup>+</sup> DISSOCIATIVE RECOMBINATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"National Institutes of Natural Sciences; National Astronomical Observatory of Japan; Eidgenössische Technische Hochschule Zürich; Stockholms Universitet; Chalmers Tekniska Högskola; National Science Council; California Institute of Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Ministry of Education, Culture, Sports, Science and Technology; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Galactic Center; Interstellar medium; Astrochemistry; Spectroscopy; Infrared; Astronomy; Galaxy","score_opus":0.010355060369009822,"score_gpt":0.22901465236066212,"score_spread":0.2186595919916523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2366293464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989209,0.000050844385,0.00020230141,0.000014084695,0.0000012146833,0.0000030901517,0.0001058487,0.000017296588,0.0006845345],"genre_scores_gemma":[0.99845624,0.000036086472,0.0006311023,0.000033826702,0.0000059394406,0.000004927502,0.00037014732,0.0000050596077,0.00045671492],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.999964,0.0000031561563,0.0000011486418,0.000012094134,0.000009862006,0.000009682553],"domain_scores_gemma":[0.9999088,0.000008287055,0.000031847703,0.000009476352,0.000011552164,0.00003008352],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010938398,0.00015636478,0.00014420236,0.0002509065,0.00040679603,0.00023941394,0.00015726357,0.00020038111,0.0012589805],"category_scores_gemma":[0.0001059778,0.00013496986,0.00009756634,0.00016926366,0.00016381017,0.00016062942,0.0001444899,0.0002669208,0.0002928416],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041749803,0.00016522055,0.45064324,0.00005340385,0.000065526,0.0006008704,0.0002643869,0.00037332333,0.5335805,0.00019228937,0.00054981414,0.0130939605],"study_design_scores_gemma":[0.000011382006,0.00010405748,0.98016596,0.000002619367,0.000011758495,0.0002841884,0.000077579796,0.0004138643,0.0180661,0.000037925514,0.0008200033,0.0000046028003],"about_ca_topic_score_codex":0.0028358356,"about_ca_topic_score_gemma":0.005347759,"teacher_disagreement_score":0.0028358356,"about_ca_system_score_codex":0.00027425875,"about_ca_system_score_gemma":0.00011417789,"threshold_uncertainty_score":0.0056385994},"labels":[],"label_agreement":null},{"id":"W2367994422","doi":"10.3847/0004-637x/832/1/26","title":"A COMPARISON AND JOINT ANALYSIS OF SUNYAEV–ZEL’DOVICH EFFECT MEASUREMENTS FROM PLANCK AND BOLOCAM FOR A SET OF 47 MASSIVE GALAXY CLUSTERS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"California Institute of Technology; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration","keywords":"Redshift; Scaling; Galaxy; Logarithm; Consistency (knowledge bases); Galaxy cluster; Planck; RADIUS; Scale (ratio)","score_opus":0.022529588090894177,"score_gpt":0.2887349098648189,"score_spread":0.26620532177392475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2367994422","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99915373,0.000021097794,0.00034927553,0.0000068017052,9.72803e-7,0.0000016316948,0.0002671564,0.000012735806,0.00018659365],"genre_scores_gemma":[0.99906176,0.000008269357,0.0002484603,0.0000031653815,0.0000022326446,0.0000029617308,0.00063544867,0.0000053790245,0.000032280608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99918145,0.00024584815,0.000047039088,0.00024752412,0.00016400509,0.000114115304],"domain_scores_gemma":[0.99648213,0.0012686461,0.0008749915,0.00079046935,0.00031174783,0.00027201633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016232923,0.00024963586,0.0003623363,0.0016231602,0.00033537636,0.0007998046,0.0005334762,0.00025534508,0.0007863119],"category_scores_gemma":[0.0039702384,0.00027063317,0.00049854326,0.00096829917,0.00037837683,0.0003352811,0.0009909332,0.0001857714,0.00018962608],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022208318,0.000016779208,0.9872295,0.000020196012,0.00043154572,0.00006196262,0.00021177263,0.0028548017,0.005132012,0.00015575826,0.00016593287,0.0034976578],"study_design_scores_gemma":[0.0000049493947,0.000021089372,0.99445033,0.0000027740987,0.00004773977,0.00002838478,0.0000739265,0.003514512,0.0016539069,0.00003331823,0.00016142258,0.0000075510798],"about_ca_topic_score_codex":0.0053482507,"about_ca_topic_score_gemma":0.005605769,"teacher_disagreement_score":0.0053482507,"about_ca_system_score_codex":0.0004607879,"about_ca_system_score_gemma":0.00016711823,"threshold_uncertainty_score":0.0106342435},"labels":[],"label_agreement":null},{"id":"W2371749441","doi":"10.3847/1538-4357/833/1/42","title":"THE IMPRINT OF RADIAL MIGRATION ON THE VERTICAL STRUCTURE OF GALAXY DISKS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Astrophysics; Galaxy; Physics; RADIUS; Scale height; Spiral galaxy; Population; Angular momentum; Geology; Spiral (railway); Astronomy; Classical mechanics; Demography","score_opus":0.0081756188290716,"score_gpt":0.21510999000594735,"score_spread":0.20693437117687574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2371749441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99574465,0.00009723896,0.0012234593,0.0001440522,0.0000133869235,0.000009155988,0.00009602281,0.000039634277,0.002632378],"genre_scores_gemma":[0.99942756,0.00002947702,0.0003470719,0.000014930067,0.0000017745293,0.0000042818947,0.000030576277,0.000009382642,0.00013500976],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998293,0.00006569069,0.000008656774,0.000018450055,0.000024716348,0.000053116983],"domain_scores_gemma":[0.9985505,0.0008031198,0.00021884768,0.0001157263,0.00015930817,0.00015261982],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004596539,0.00039100175,0.00031373877,0.00040171802,0.0006126089,0.0009092253,0.0005155344,0.0007499976,0.0011832888],"category_scores_gemma":[0.0040932274,0.00027714515,0.00043350132,0.00028997447,0.0007311932,0.0006218179,0.00066437287,0.0005442916,0.00013848669],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002420757,0.000107621316,0.035225514,0.00004830634,0.0000586021,0.00035059536,0.00014984864,0.9504001,0.0077228514,0.0028332802,0.00033610294,0.0025251245],"study_design_scores_gemma":[0.000046025976,0.00014131966,0.00868523,0.000019043762,0.000020955771,0.00003798195,0.00014140311,0.9882306,0.0015558623,0.00084957975,0.00025250006,0.000019527712],"about_ca_topic_score_codex":0.018155826,"about_ca_topic_score_gemma":0.008250752,"teacher_disagreement_score":0.018155826,"about_ca_system_score_codex":0.0008617616,"about_ca_system_score_gemma":0.00046649307,"threshold_uncertainty_score":0.03610027},"labels":[],"label_agreement":null},{"id":"W2375094142","doi":"10.3847/0004-637x/825/2/83","title":"COMPARING SIMULATIONS OF AGN FEEDBACK","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science and Technology Facilities Council","keywords":"Virial theorem; Smoothed-particle hydrodynamics; Radiative cooling; Halo; Star formation; Adaptive mesh refinement; Accretion (finance); Galaxy; Baryon","score_opus":0.01424168937841167,"score_gpt":0.22685293257877143,"score_spread":0.21261124320035976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2375094142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.987362,0.00013411022,0.0038422195,0.00023961168,0.000047898844,0.000030170326,0.00052195985,0.00059069303,0.00723131],"genre_scores_gemma":[0.9942135,0.00004403195,0.0043465667,0.00007524229,0.000013649753,0.000024715895,0.0004670014,0.00009566419,0.00071966473],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997069,0.000090500405,0.000015515088,0.000051332463,0.00006998713,0.00006577919],"domain_scores_gemma":[0.9986695,0.0007268901,0.00011473443,0.00016110875,0.0001944772,0.00013325442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005526659,0.0004811899,0.0006339152,0.00047963456,0.0004091138,0.0007057129,0.0012615938,0.0010155544,0.002174988],"category_scores_gemma":[0.0028295896,0.0002330314,0.0006319013,0.00044706435,0.00058781996,0.00048589954,0.0006603625,0.00062623626,0.00023260187],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030947922,0.00021405189,0.00936606,0.00009827769,0.000099892764,0.00017295267,0.00016206328,0.9755347,0.0056236866,0.0023457194,0.00077583926,0.0052972496],"study_design_scores_gemma":[0.000055042565,0.00007302811,0.001844944,0.00000630073,0.00001114137,0.000018473806,0.00003462785,0.99586856,0.0012684759,0.00043285787,0.0003746162,0.000011979557],"about_ca_topic_score_codex":0.01785485,"about_ca_topic_score_gemma":0.008214661,"teacher_disagreement_score":0.01785485,"about_ca_system_score_codex":0.0008148141,"about_ca_system_score_gemma":0.0006056611,"threshold_uncertainty_score":0.035501838},"labels":[],"label_agreement":null},{"id":"W2375373748","doi":"10.3847/0004-637x/826/1/46","title":"THE ENVIRONMENT OF z &gt; 1 3CR RADIO GALAXIES AND QSOS: FROM PROTO-CLUSTERS TO CLUSTERS OF GALAXIES?","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Cluster (spacecraft); Galaxy; Galaxy cluster; RADIUS; Active galactic nucleus; Radio galaxy; Population; Position (finance)","score_opus":0.005638781006856349,"score_gpt":0.19035306911846894,"score_spread":0.18471428811161258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2375373748","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938107,0.000062455736,0.00004708161,0.000021433012,4.2891887e-7,0.0000013685852,0.00009992236,0.0000032836256,0.00038294896],"genre_scores_gemma":[0.99981064,0.000020513298,0.00002711257,0.0000063690845,0.00000161032,5.47609e-7,0.00006529672,0.0000014640655,0.00006650336],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979085,0.000033532895,0.0000084386265,0.00006168737,0.000039127877,0.000066378605],"domain_scores_gemma":[0.99931085,0.00008562413,0.00031240686,0.00005111164,0.00008479373,0.00015524207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027128417,0.00012244354,0.00023122343,0.0010469416,0.00036198704,0.000729946,0.0002521021,0.00018429365,0.0013933822],"category_scores_gemma":[0.00071498606,0.00009438743,0.00011536159,0.0010301052,0.0006424448,0.00036514417,0.0005310478,0.00012145974,0.00029378737],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000824521,0.000016212556,0.9943585,0.000006016166,0.000014630952,0.00007317415,0.0002499845,0.00014804935,0.0026653,0.00023874012,0.00011393635,0.0020330867],"study_design_scores_gemma":[0.0000010580819,0.0000085829415,0.99946755,0.0000010004562,0.0000039922415,0.000036579797,0.0001352332,0.00012396036,0.00009139356,0.000038389226,0.00009116367,0.0000011436994],"about_ca_topic_score_codex":0.019742513,"about_ca_topic_score_gemma":0.021314073,"teacher_disagreement_score":0.019742513,"about_ca_system_score_codex":0.00040267635,"about_ca_system_score_gemma":0.00016351833,"threshold_uncertainty_score":0.0392552},"labels":[],"label_agreement":null},{"id":"W2376456712","doi":"10.3847/0004-637x/828/1/3","title":"ASASSN-15LH: A SUPERLUMINOUS ULTRAVIOLET REBRIGHTENING OBSERVED BY SWIFT AND HUBBLE*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Space Telescope Science Institute; McMaster University; National Aeronautics and Space Administration","keywords":"Redshift; Photometry (optics); Supernova; Ultraviolet; Spectral line; Emission spectrum; Spectroscopy; Polarimetry; Stars","score_opus":0.012613432052039398,"score_gpt":0.21003235784119614,"score_spread":0.19741892578915674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2376456712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989536,0.000054934393,0.00005534646,0.0000168378,0.000006181593,0.0000050299677,0.00012698748,0.000013106653,0.00076801796],"genre_scores_gemma":[0.9991192,0.000016738215,0.0000960116,0.00003341262,0.000008521027,0.0000029106745,0.00033698409,0.0000033679898,0.0003827652],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999099,0.0000051493203,0.000007486403,0.000024137911,0.000022490192,0.000030730305],"domain_scores_gemma":[0.9996271,0.000015502226,0.00011324859,0.000026854144,0.00002780304,0.00018951124],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016184691,0.00029671256,0.00033426713,0.000775039,0.00043911109,0.00033204065,0.00027296433,0.00027336046,0.0014790412],"category_scores_gemma":[0.00016478694,0.00012120591,0.0002336813,0.0003551844,0.00029854593,0.00017575748,0.0004942672,0.00029633968,0.00032010567],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040172832,0.00015834274,0.9617613,0.000024876183,0.000060539962,0.0024116023,0.00045520716,0.00011514737,0.02507986,0.00012359578,0.00079686014,0.0086109955],"study_design_scores_gemma":[0.0000074067193,0.00014601772,0.9966647,0.000004917952,0.000007633181,0.0010402129,0.00014874325,0.00016374183,0.00075824047,0.000027766631,0.0010270342,0.0000036700415],"about_ca_topic_score_codex":0.0055928417,"about_ca_topic_score_gemma":0.011951989,"teacher_disagreement_score":0.0055928417,"about_ca_system_score_codex":0.00030330403,"about_ca_system_score_gemma":0.00012224614,"threshold_uncertainty_score":0.011120617},"labels":[],"label_agreement":null},{"id":"W2379470424","doi":"10.3847/0004-637x/826/1/8","title":"EXTRASOLAR STORMS: PRESSURE-DEPENDENT CHANGES IN LIGHT-CURVE PHASE IN BROWN DWARFS FROM SIMULTANEOUS HST AND SPITZER OBSERVATIONS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Western University","funders":"","keywords":"Light curve; Brown dwarf; Grism; Flux (metallurgy); Wavelength; Photometry (optics); Spectral line; Phase (matter); Fourier analysis","score_opus":0.016602881422716237,"score_gpt":0.23759374074561504,"score_spread":0.2209908593228988,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2379470424","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991736,0.000022727854,0.00021684828,0.0000090936865,0.0000015583583,0.0000035114963,0.0002426724,0.0000292011,0.00030071335],"genre_scores_gemma":[0.99913365,0.000017167751,0.00019660027,0.0000055948926,0.0000058332284,0.0000030085707,0.0005492539,0.000008215274,0.00008080534],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991727,0.00000929745,0.00000493061,0.000019338446,0.00003116286,0.000018084507],"domain_scores_gemma":[0.9996076,0.000061658015,0.00011890278,0.00003652681,0.00007279828,0.000102426726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023470554,0.00018432458,0.00022363206,0.001017016,0.00023835164,0.00031350824,0.000166604,0.00025769297,0.0006131498],"category_scores_gemma":[0.0006155528,0.00014585102,0.00019753033,0.00055425667,0.00018633429,0.00023500674,0.00031088336,0.00018382644,0.00019122133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003577051,0.000067852314,0.9159798,0.000032007363,0.00007188948,0.0002616989,0.0003467263,0.0018857905,0.07073244,0.00008157946,0.0003621267,0.009820498],"study_design_scores_gemma":[0.0000026101052,0.000016182954,0.99812704,8.655946e-7,0.0000046927266,0.000046825186,0.00002506491,0.0008957657,0.0007963246,0.000015837393,0.000066627006,0.0000020822597],"about_ca_topic_score_codex":0.004494316,"about_ca_topic_score_gemma":0.009224815,"teacher_disagreement_score":0.004494316,"about_ca_system_score_codex":0.0002545694,"about_ca_system_score_gemma":0.00011352283,"threshold_uncertainty_score":0.008936286},"labels":[],"label_agreement":null},{"id":"W2394833128","doi":"10.3847/0004-637x/825/2/114","title":"THE MURCHISON WIDEFIELD ARRAY 21 cm POWER SPECTRUM ANALYSIS METHODOLOGY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"U.S. Air Force; Victoria University; Smithsonian Astrophysical Observatory; Astronomy Australia Limited; Victoria University of Wellington; Ministero dello Sviluppo Economico; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Curtin University of Technology; Smithsonian Institution; Nvidia; Harvard University; National Science Foundation","keywords":"Reionization; Spectral density; Statistical power; Pipeline (software); Spectral line; Redshift; Calibration; Range (aeronautics); Murchison meteorite","score_opus":0.018259278550627527,"score_gpt":0.25780970054216334,"score_spread":0.2395504219915358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2394833128","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.023726203,0.0002830798,0.9521114,0.00030959662,0.00007732346,0.0003893814,0.0014517347,0.002076369,0.019574957],"genre_scores_gemma":[0.1482072,0.00021652154,0.8390175,0.00021957792,0.00013635439,0.0006277903,0.0018944242,0.00064122817,0.009039287],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9984285,0.00042223997,0.000065981,0.00038793168,0.0005517314,0.00014354652],"domain_scores_gemma":[0.99784636,0.0004425678,0.00029744336,0.00053606834,0.00078278274,0.00009471342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026588836,0.00076108245,0.00034538112,0.0035073962,0.0008262435,0.0016428541,0.0012909706,0.00046865584,0.010060771],"category_scores_gemma":[0.0066362484,0.00035801352,0.0006592705,0.0021880309,0.0006589621,0.0010118069,0.0018199933,0.00075084186,0.0028650642],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026582758,0.000106215746,0.05185006,0.00035203874,0.0002720452,0.0006348583,0.0011221995,0.028083485,0.053904478,0.15890594,0.022190286,0.6823126],"study_design_scores_gemma":[0.00013650327,0.0003725173,0.16020069,0.00023121898,0.00016334248,0.0020736824,0.0012119295,0.3045478,0.06228579,0.19732442,0.27116418,0.0002879178],"about_ca_topic_score_codex":0.0066449773,"about_ca_topic_score_gemma":0.005403814,"teacher_disagreement_score":0.010060771,"about_ca_system_score_codex":0.001011522,"about_ca_system_score_gemma":0.0018176126,"threshold_uncertainty_score":0.033656597},"labels":[],"label_agreement":null},{"id":"W2395159461","doi":"10.3847/1538-4357/aa62a7","title":"Comparing Submillimeter Polarized Emission with Near-infrared Polarization of Background Stars for the Vela C Molecular Cloud","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"HORIZON EUROPE Marie Sklodowska-Curie Actions; Science and Technology Facilities Council; Canadian Space Agency; Horizon 2020 Framework Programme; Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; European Commission; National Aeronautics and Space Administration; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Office of Polar Programs; Leverhulme Trust; Illinois Space Grant Consortium; Ontario Innovation Trust; National Science Foundation","keywords":"Vela; Polarization (electrochemistry); Starlight; Molecular cloud; Stars; Telescope; Interstellar medium; Cosmic dust","score_opus":0.02137651636642981,"score_gpt":0.26098657581049717,"score_spread":0.23961005944406735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2395159461","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978021,0.0000694274,0.00045118862,0.000010311258,0.0000028757404,0.0000069739053,0.00096815056,0.000026699036,0.0006623321],"genre_scores_gemma":[0.99731797,0.000030531763,0.000442913,0.000012466037,0.0000062512618,0.0000057586467,0.0021214264,0.000011516245,0.000051090916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995735,0.000048102876,0.000022088687,0.00012453327,0.00012628875,0.000105533705],"domain_scores_gemma":[0.9988921,0.00026951902,0.00029633782,0.00014131023,0.00021405464,0.00018663643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005644985,0.00032317726,0.00024549747,0.0023080725,0.00052087713,0.00075599004,0.00042119608,0.00034491697,0.0007002081],"category_scores_gemma":[0.0011256895,0.00022802569,0.0004440992,0.0012274816,0.000163983,0.0003282377,0.0005499539,0.00029626992,0.0002966215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019435829,0.00008689124,0.9625216,0.00002858371,0.00018141237,0.000099110905,0.000096722164,0.0019841578,0.02762725,0.00009452612,0.00029433047,0.0067910757],"study_design_scores_gemma":[0.0000060902516,0.000026688971,0.99411076,0.0000046543614,0.000029647243,0.000036641875,0.000050215836,0.0024558841,0.0030376385,0.000022725044,0.00021344917,0.000005605308],"about_ca_topic_score_codex":0.008872441,"about_ca_topic_score_gemma":0.015102438,"teacher_disagreement_score":0.008872441,"about_ca_system_score_codex":0.00038425747,"about_ca_system_score_gemma":0.00018940221,"threshold_uncertainty_score":0.017641604},"labels":[],"label_agreement":null},{"id":"W2396677916","doi":"10.3847/0004-637x/827/1/30","title":"APPLICATION OF A THEORY AND SIMULATION-BASED CONVECTIVE BOUNDARY MIXING MODEL FOR AGB STAR EVOLUTION AND NUCLEOSYNTHESIS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Convection; Nucleosynthesis; Mixing (physics); Convective mixing; Stellar evolution; Envelope (radar); Convection zone; Stars","score_opus":0.008433242271453813,"score_gpt":0.22911320244852548,"score_spread":0.22067996017707167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2396677916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75456965,0.0005905749,0.21336818,0.0012065262,0.00020493277,0.00020596552,0.00050659064,0.0004881683,0.028859498],"genre_scores_gemma":[0.9836331,0.00012055781,0.013610613,0.000056386627,0.00004752584,0.00015146867,0.00011710487,0.000047587473,0.0022155426],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998598,0.000058521815,0.000007109461,0.000021406808,0.000028331298,0.000024722123],"domain_scores_gemma":[0.9996326,0.00012932603,0.00006366752,0.00003204886,0.00007241669,0.00006992336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037167128,0.00069758156,0.00075144414,0.0004837278,0.0008513749,0.0009593263,0.001207865,0.0012768935,0.0018850133],"category_scores_gemma":[0.0009840628,0.00040921723,0.0009116221,0.0004070024,0.00081665214,0.0005945938,0.0009567145,0.00067382527,0.00020412917],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022573257,0.000026423273,0.0005841165,0.000009415643,0.000014130349,0.00004138413,0.000016500873,0.9928779,0.001216447,0.0045450344,0.00008420178,0.0005618998],"study_design_scores_gemma":[0.000008004094,0.000005384976,0.00007714074,8.68217e-7,0.0000017141176,0.0000019796921,0.0000016845439,0.9993262,0.0000725114,0.00043215475,0.0000705661,0.0000018474525],"about_ca_topic_score_codex":0.024356969,"about_ca_topic_score_gemma":0.0058393874,"teacher_disagreement_score":0.024356969,"about_ca_system_score_codex":0.0013887514,"about_ca_system_score_gemma":0.0012028688,"threshold_uncertainty_score":0.048430383},"labels":[],"label_agreement":null},{"id":"W2396866467","doi":"10.3847/0004-637x/826/1/95","title":"THE JCMT GOULD BELT SURVEY: EVIDENCE FOR DUST GRAIN EVOLUTION IN PERSEUS STAR-FORMING CLUMPS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Manitoba; University of Waterloo; Herzberg Institute of Astrophysics; University of Alberta; Université Laval; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Molecular cloud; Emissivity; Stars; Cosmic dust; Spectral energy distribution; Mass distribution; Extinction (optical mineralogy); Optical depth","score_opus":0.03852589389507161,"score_gpt":0.2954560419134942,"score_spread":0.2569301480184226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2396866467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991769,0.000071358445,0.000037311092,0.000013503815,0.0000010707615,0.0000022733793,0.00035905806,0.000008739606,0.0003297008],"genre_scores_gemma":[0.99945503,0.00002993119,0.000075347896,0.000010107361,0.000002310468,0.0000014968921,0.0003452963,0.0000023826374,0.0000780794],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998951,0.000009286185,0.0000071593604,0.000040975654,0.000025901818,0.00002163173],"domain_scores_gemma":[0.9995448,0.0000503786,0.00018695583,0.000039958853,0.00007688063,0.000101024925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016306492,0.00019409171,0.00015269333,0.0018680327,0.00021163802,0.00035312385,0.0002555338,0.00015902985,0.0008892184],"category_scores_gemma":[0.00045131083,0.000091848466,0.000093369235,0.0009145749,0.00027772418,0.0001680056,0.0003588854,0.000086517466,0.00017881097],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003275501,0.0000073112446,0.993294,0.000008400966,0.000016627457,0.00011138407,0.00014846926,0.00007641835,0.003945404,0.000036838584,0.00015876604,0.0021635569],"study_design_scores_gemma":[0.0000013226154,0.0000034689044,0.999566,0.0000018624813,0.0000017024377,0.000047226324,0.00006907631,0.0000665848,0.00013369763,0.000006431633,0.00010211281,5.079654e-7],"about_ca_topic_score_codex":0.024363503,"about_ca_topic_score_gemma":0.027731877,"teacher_disagreement_score":0.024363503,"about_ca_system_score_codex":0.00033721342,"about_ca_system_score_gemma":0.00012379706,"threshold_uncertainty_score":0.048443437},"labels":[],"label_agreement":null},{"id":"W2398084842","doi":"10.3847/0004-637x/825/1/32","title":"FAR INFRARED VARIABILITY OF SAGITTARIUS A*: 25.5 hr OF MONITORING WITH HERSCHEL*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"European Space Agency; Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Spectral energy distribution; Accretion (finance); Supermassive black hole; Light curve; Black hole (networking); Wavelength; Sagittarius A*; Maser; Infrared","score_opus":0.012316149829035436,"score_gpt":0.22604914344685284,"score_spread":0.2137329936178174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2398084842","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955722,0.000069843256,0.0002511102,0.00003791522,0.000005566948,0.000005307573,0.0024802485,0.00010711398,0.001470752],"genre_scores_gemma":[0.99521834,0.000028066866,0.00044789107,0.000025529496,0.0000127196345,0.0000054586917,0.0037941725,0.000009318992,0.0004585219],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988973,0.00000942354,0.000004765999,0.000040330127,0.000030710115,0.000025003937],"domain_scores_gemma":[0.999788,0.000016958074,0.0000726543,0.000028750093,0.000040961455,0.000052567877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019119836,0.00018143817,0.00014203867,0.0007369512,0.00018053029,0.00027100212,0.00018532874,0.00024060524,0.00095880183],"category_scores_gemma":[0.00023997886,0.000074160416,0.00014788668,0.0003736346,0.00009189806,0.00019344174,0.00026940595,0.00018243706,0.00040949468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018496421,0.00010856845,0.94264054,0.000025925108,0.00016188256,0.00018430005,0.00018093595,0.0011059059,0.037791327,0.00014330339,0.0022274146,0.015244918],"study_design_scores_gemma":[0.0000013840951,0.000017327468,0.99814236,0.0000014039634,0.0000055198784,0.00003132406,0.000023305496,0.00037533548,0.0008816827,0.000009386595,0.00050866517,0.000002291174],"about_ca_topic_score_codex":0.0057872464,"about_ca_topic_score_gemma":0.012657469,"teacher_disagreement_score":0.0057872464,"about_ca_system_score_codex":0.00027475733,"about_ca_system_score_gemma":0.000081912374,"threshold_uncertainty_score":0.0115071535},"labels":[],"label_agreement":null},{"id":"W2398434821","doi":"10.3847/0004-637x/826/2/158","title":"A STUDY OF THE ELEMENTS COPPER THROUGH URANIUM IN SIRIUS A: CONTRIBUTIONS FROM STIS AND GROUND-BASED SPECTRA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University","funders":"","keywords":"Spectrograph; Sirius; Physics; Astrophysics; Space Telescope Imaging Spectrograph; Stars; Astronomy; Spectral line; Sky; Hubble space telescope","score_opus":0.012795458908065023,"score_gpt":0.24531488548811273,"score_spread":0.2325194265800477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2398434821","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986687,0.000055787186,0.00012493528,0.0000041047915,8.010893e-7,0.0000014614744,0.00021296495,0.000009403975,0.0009219264],"genre_scores_gemma":[0.9985708,0.000039888022,0.00043760074,0.0000038247777,0.000004318338,0.0000014028952,0.0006520512,0.000010649255,0.00027951546],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998435,0.000024537148,0.000009801881,0.000052875996,0.00004917134,0.000020061081],"domain_scores_gemma":[0.9994771,0.00012452745,0.00014686694,0.000053570333,0.00013020553,0.000067706205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028593908,0.00024014068,0.0002301075,0.0017895959,0.00027676782,0.0004917521,0.00021331363,0.00015199954,0.00083814195],"category_scores_gemma":[0.00056328834,0.00016026011,0.00021887725,0.0009005217,0.00020572789,0.0002280309,0.00045970318,0.00012299704,0.0004365322],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033174243,0.00004278456,0.9289554,0.000073027404,0.00010300312,0.00024233948,0.00052120275,0.000877288,0.056532435,0.00026744942,0.00022627893,0.011827175],"study_design_scores_gemma":[0.000007869188,0.00014257856,0.9853496,0.000013716165,0.00003710991,0.00022736845,0.0003426291,0.0034692357,0.009072393,0.000058607897,0.0012724795,0.000006449221],"about_ca_topic_score_codex":0.002781565,"about_ca_topic_score_gemma":0.004294086,"teacher_disagreement_score":0.002781565,"about_ca_system_score_codex":0.0001906475,"about_ca_system_score_gemma":0.00009731101,"threshold_uncertainty_score":0.0055307746},"labels":[],"label_agreement":null},{"id":"W2398661772","doi":"10.3847/0004-637x/826/1/63","title":"EXPECTATION ON OBSERVATION OF SUPERNOVA REMNANTS WITH THE LHAASO PROJECT","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Observatory; Crab Nebula; Cosmic ray; Supernova; Sky; Air shower; Particle acceleration; Acceleration","score_opus":0.018169574221833757,"score_gpt":0.2357220736114033,"score_spread":0.21755249938956953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2398661772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9724053,0.0007443906,0.002528982,0.0004857215,0.00007714301,0.00012793731,0.007925663,0.0005466981,0.0151581345],"genre_scores_gemma":[0.9846603,0.00026095464,0.0035699443,0.00019480324,0.00008230369,0.000045541838,0.008484106,0.000042332336,0.00265973],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99923813,0.0001753259,0.0000392626,0.00015758644,0.00025561807,0.00013399709],"domain_scores_gemma":[0.997609,0.00025528047,0.00045744938,0.0003191417,0.0005714031,0.0007875695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00209249,0.00041882263,0.00020701872,0.001765724,0.00048692233,0.0009409398,0.00031777864,0.00032841388,0.0021682945],"category_scores_gemma":[0.0013986842,0.00015063246,0.0003618478,0.0006653227,0.00035790825,0.0003659605,0.0014385326,0.00030621592,0.00079612463],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005207581,0.00015679447,0.96454686,0.0000562037,0.000098121345,0.0006472292,0.00022511452,0.00032046955,0.008166142,0.0005558264,0.0027987314,0.02190778],"study_design_scores_gemma":[0.000026115735,0.0002741395,0.9826545,0.000022767712,0.000056401328,0.0006859971,0.00026263358,0.00081660185,0.0025860795,0.00029763972,0.012302365,0.0000148191175],"about_ca_topic_score_codex":0.006285871,"about_ca_topic_score_gemma":0.008389969,"teacher_disagreement_score":0.006285871,"about_ca_system_score_codex":0.00047956116,"about_ca_system_score_gemma":0.00051372166,"threshold_uncertainty_score":0.012498558},"labels":[],"label_agreement":null},{"id":"W2398732896","doi":"10.3847/0004-637x/825/2/146","title":"CHEMICAL TAGGING IN THE SDSS-III/APOGEE SURVEY: NEW IDENTIFICATIONS OF HALO STARS WITH GLOBULAR CLUSTER ORIGINS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Ministerio de Economía y Competitividad; York University; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Office of Science; Johns Hopkins University; Science and Technology Facilities Council; Carnegie Mellon University; College of Engineering, Michigan State University; Magyar Tudományos Akadémia; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Globular cluster; Halo; Galactic halo; Horizontal branch; Stars; Sky; Population; Blue straggler","score_opus":0.015257791543389144,"score_gpt":0.2368624083286946,"score_spread":0.22160461678530546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2398732896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988385,0.00016282503,0.0001334708,0.00003370772,0.0000023469488,0.0000022700985,0.00025108038,0.000008131033,0.00056757964],"genre_scores_gemma":[0.9989593,0.00010592043,0.000252913,0.00003355412,0.0000063804705,0.0000021553287,0.00047951753,0.000003383953,0.00015682416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971527,0.00004318287,0.000025410704,0.000075718504,0.00008867017,0.000051759238],"domain_scores_gemma":[0.9982186,0.000289715,0.00063730346,0.00022758389,0.00031273306,0.00031406246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00091962557,0.00016717783,0.00022211987,0.003064205,0.0002842094,0.0006459428,0.00025909994,0.000263349,0.00083712663],"category_scores_gemma":[0.0014106655,0.00015417009,0.00018080021,0.0017333984,0.00051172986,0.0005169619,0.0010423135,0.0001818183,0.0002907091],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000038278544,0.0000066708403,0.99520594,0.0000067831315,0.000017960789,0.00003835378,0.00013882788,0.000032001593,0.0023719755,0.000053149157,0.000088169916,0.0020019289],"study_design_scores_gemma":[0.0000016175188,0.000005308654,0.9993284,0.0000025731026,0.0000055933947,0.000044681852,0.000118797034,0.00006903539,0.00019481884,0.00004034464,0.00018714993,0.0000017199475],"about_ca_topic_score_codex":0.0050982554,"about_ca_topic_score_gemma":0.010998187,"teacher_disagreement_score":0.0050982554,"about_ca_system_score_codex":0.0003065577,"about_ca_system_score_gemma":0.00018100963,"threshold_uncertainty_score":0.010137141},"labels":[],"label_agreement":null},{"id":"W2399110274","doi":"10.3847/0004-637x/826/1/88","title":"DYNAMICAL ESTIMATE OF POST-MAIN-SEQUENCE STELLAR MASSES IN 47 TUCANAE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"Physics; Stars; Astrophysics; Red-giant branch; Asymptotic giant branch; Blue straggler; Horizontal branch; Astronomy; Population; Globular cluster; Mass segregation; Stellar mass loss; Sequence (biology); Stellar evolution; Biology","score_opus":0.011146197596674425,"score_gpt":0.24566778583766685,"score_spread":0.23452158824099242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2399110274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984901,0.00011061492,0.00030848154,0.000011025183,0.0000016380457,0.0000036698511,0.00026340623,0.000012532226,0.0007983997],"genre_scores_gemma":[0.9986559,0.00003222884,0.00033840147,0.0000054747,0.0000016420436,0.000004235102,0.0006825696,0.0000060083394,0.0002735037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998338,0.000009048137,0.0000062155455,0.000048965016,0.000043710665,0.00005823591],"domain_scores_gemma":[0.9994771,0.00006730846,0.00010351903,0.00004602654,0.0002059853,0.00010004496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026204664,0.00023351381,0.0002940174,0.0016509929,0.0007493629,0.00071613444,0.0005233363,0.0003683427,0.001122439],"category_scores_gemma":[0.0010245865,0.00012628092,0.00022789527,0.0009853701,0.00026992144,0.00023248058,0.00051582616,0.00022256508,0.0003113339],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014114726,0.000019640427,0.9712511,0.000011688085,0.00006079556,0.000063486834,0.00023192288,0.0024776228,0.014856228,0.00022417893,0.00011729709,0.010544956],"study_design_scores_gemma":[0.0000014635888,0.000012419048,0.99527234,0.000002575785,0.000010243375,0.000023698563,0.000080553255,0.0021791754,0.0019117884,0.000040600207,0.00046163844,0.000003526228],"about_ca_topic_score_codex":0.11133983,"about_ca_topic_score_gemma":0.12214307,"teacher_disagreement_score":0.11133983,"about_ca_system_score_codex":0.0019289927,"about_ca_system_score_gemma":0.0005276544,"threshold_uncertainty_score":0.22138351},"labels":[],"label_agreement":null},{"id":"W2401842760","doi":"10.3847/0004-637x/823/1/23","title":"NUMERICAL TEST OF DIFFERENT APPROXIMATIONS USED IN THE TRANSPORT THEORY OF ENERGETIC PARTICLES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Test particle; Gyroradius; Diffusion; Statistical physics; Nonlinear system; Work (physics); Guiding center; Taylor series; Classical mechanics; Mathematical analysis; Quantum mechanics; Plasma; Mathematics","score_opus":0.008828235151606962,"score_gpt":0.2131893404251068,"score_spread":0.20436110527349982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2401842760","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98300505,0.00013429986,0.0126173515,0.00022477913,0.000046040794,0.000030180416,0.00010691502,0.00011165706,0.0037237909],"genre_scores_gemma":[0.99261993,0.000048916987,0.0067996336,0.000017958351,0.0000066705393,0.000020549336,0.00007640801,0.000022585004,0.00038745196],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99973446,0.000099772835,0.000020023192,0.000022752587,0.000075292664,0.00004768253],"domain_scores_gemma":[0.9971307,0.0018487908,0.00030289646,0.00028214348,0.00032771914,0.00010783392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009181416,0.0004183663,0.0005012636,0.0005155811,0.00053719705,0.0006582368,0.00088984176,0.00076620263,0.00067111215],"category_scores_gemma":[0.0045047887,0.00013226742,0.0003455769,0.00060162746,0.0007446961,0.000556372,0.00060413615,0.00075063296,0.00007371277],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035629582,0.00032012156,0.009887125,0.0001249283,0.00006920395,0.00034136206,0.00019363008,0.9458709,0.008907787,0.027250612,0.0005673303,0.006110773],"study_design_scores_gemma":[0.000016872184,0.0000393003,0.00040564922,0.0000037481855,0.000004131057,0.000010673535,0.000015368907,0.9972127,0.001604269,0.00059806847,0.000084365434,0.0000049223554],"about_ca_topic_score_codex":0.0105189765,"about_ca_topic_score_gemma":0.003575534,"teacher_disagreement_score":0.0105189765,"about_ca_system_score_codex":0.0006430314,"about_ca_system_score_gemma":0.0005946366,"threshold_uncertainty_score":0.020915508},"labels":[],"label_agreement":null},{"id":"W2405552219","doi":"10.3847/0004-637x/818/2/103","title":"PLANETARY EMBRYO BOW SHOCKS AS A MECHANISM FOR CHONDRULE FORMATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Planetary Science and Exploration","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Bow shock (aerodynamics); Chondrule; Radiative transfer; Outgassing; Shock (circulatory); Bow wave; Thermal; Radiative cooling; Shock wave","score_opus":0.011919175350886348,"score_gpt":0.2174278275680216,"score_spread":0.20550865221713524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2405552219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868782,0.00007715233,0.0066067073,0.00012593348,0.000022640144,0.00003321554,0.00008403888,0.00011596536,0.0060562184],"genre_scores_gemma":[0.99896884,0.000024210756,0.000565328,0.000017760736,0.0000043005093,0.000006957586,0.000020678266,0.0000102394615,0.00038162552],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989593,0.000024433797,0.0000040738573,0.000012681275,0.000025805779,0.00003712993],"domain_scores_gemma":[0.999736,0.00008271376,0.000053980737,0.000035002176,0.000028961258,0.00006333882],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025871905,0.00032725531,0.0004339741,0.00024794342,0.00054364477,0.0009768881,0.0008134875,0.0005484575,0.0029826488],"category_scores_gemma":[0.0010981335,0.00026445006,0.00056622043,0.00015958458,0.00062888564,0.0005105328,0.0009295723,0.00057713763,0.00016073683],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002927014,0.00011619309,0.02945677,0.00006417636,0.00012692157,0.0010405459,0.0001801557,0.92087585,0.019706294,0.02387471,0.0005194051,0.003746317],"study_design_scores_gemma":[0.0001809102,0.00018203042,0.010081342,0.00001068501,0.000035319285,0.00010558146,0.00011329171,0.9798226,0.0051222723,0.0036844134,0.00063968287,0.00002186542],"about_ca_topic_score_codex":0.006975369,"about_ca_topic_score_gemma":0.0022311618,"teacher_disagreement_score":0.006975369,"about_ca_system_score_codex":0.00079895527,"about_ca_system_score_gemma":0.0005260833,"threshold_uncertainty_score":0.013869584},"labels":[],"label_agreement":null},{"id":"W2406580827","doi":"10.3847/0004-637x/832/2/196","title":"DEPENDENCE OF SMALL PLANET FREQUENCY ON STELLAR METALLICITY HIDDEN BY THEIR PREVALENCE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"","keywords":"Planet; Metallicity; Stars; Exoplanet; Planetary system; Correlation; Asteroseismology; Gas giant","score_opus":0.01458881168967367,"score_gpt":0.21237235536411608,"score_spread":0.19778354367444242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2406580827","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954072,0.0002491694,0.0016644205,0.00006302242,0.0000052502787,0.000004549335,0.00027630743,0.000035049736,0.002295087],"genre_scores_gemma":[0.9997433,0.00001665147,0.00006629852,0.0000046882424,0.0000031759437,7.872145e-7,0.00007084523,0.0000039572856,0.00009022516],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99908674,0.0002296303,0.00006246903,0.00038356433,0.00012761522,0.00011000711],"domain_scores_gemma":[0.96660167,0.0235321,0.004956051,0.002725047,0.0010120159,0.0011731134],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012433644,0.00015601434,0.00033850197,0.0011470043,0.00030559037,0.00087642466,0.0003807369,0.00051625527,0.004414709],"category_scores_gemma":[0.015880758,0.00021348658,0.00028161707,0.00056209555,0.00072827906,0.0007824744,0.0006058545,0.00042055736,0.00078341115],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014512594,0.000010929527,0.991958,0.000018389315,0.000065522654,0.00008902204,0.00007459651,0.000559797,0.0031799325,0.00036666286,0.00007502959,0.0034570007],"study_design_scores_gemma":[0.0000037977738,0.000054751225,0.99329066,0.000005497173,0.000026044296,0.00047126476,0.00006478979,0.0036209878,0.001504908,0.0006985207,0.00025334727,0.0000053817403],"about_ca_topic_score_codex":0.0008712358,"about_ca_topic_score_gemma":0.0005726243,"teacher_disagreement_score":0.004414709,"about_ca_system_score_codex":0.00018700566,"about_ca_system_score_gemma":0.000103624014,"threshold_uncertainty_score":0.01476866},"labels":[],"label_agreement":null},{"id":"W2411647658","doi":"10.3847/0004-637x/826/2/202","title":"MAGNETIC FIELD STRENGTH IN AN INTERMEDIATE-VELOCITY IONIZED FILAMENT IN THE FIRST GALACTIC QUADRANT","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Faraday effect; Magnetic field; Protein filament; Faraday cage; Astrophysics; Galaxy; Field strength; Plasma; Drift velocity; Measure (data warehouse); Velocity dispersion; Rotation (mathematics); Interstellar medium; Computational physics; Geometry; Nuclear physics; Quantum mechanics","score_opus":0.007285061034451187,"score_gpt":0.217136232815321,"score_spread":0.20985117178086982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2411647658","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99947935,0.000029937459,0.000049496637,0.000009092436,2.6641604e-7,5.1389e-7,0.000027159293,0.0000022794695,0.00040195245],"genre_scores_gemma":[0.9998907,0.000007830299,0.000027734939,0.0000017938635,8.112687e-7,3.8524476e-7,0.00004241016,6.311193e-7,0.00002771812],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995255,0.000007961158,0.0000021317305,0.00001051345,0.0000072117305,0.000019726727],"domain_scores_gemma":[0.9996692,0.0000760408,0.0001341791,0.00001608569,0.00004193745,0.000062604006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011057332,0.000093561575,0.00014548072,0.0008935308,0.00023188046,0.00054493634,0.00024646844,0.00014735572,0.00073442905],"category_scores_gemma":[0.0005206406,0.0000624144,0.0001027873,0.0004440067,0.0002959052,0.00016674498,0.00027287533,0.00010569693,0.00010448658],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032194826,0.000033289754,0.9563038,0.000017514116,0.00004492032,0.0007240083,0.0003778029,0.0018463716,0.034883708,0.0012606456,0.00015790315,0.0040280935],"study_design_scores_gemma":[0.00000576205,0.00002866385,0.9971378,0.0000037607147,0.000010039644,0.0001866939,0.0001297538,0.0012030414,0.00096848275,0.00015069744,0.00017160235,0.0000036942909],"about_ca_topic_score_codex":0.0060762316,"about_ca_topic_score_gemma":0.0037081318,"teacher_disagreement_score":0.0060762316,"about_ca_system_score_codex":0.00050942594,"about_ca_system_score_gemma":0.0000554657,"threshold_uncertainty_score":0.012081683},"labels":[],"label_agreement":null},{"id":"W2413936025","doi":"10.3847/0004-637x/824/1/62","title":"ERRATUM: “BLACK HOLE–NEUTRON STAR MERGERS WITH A HOT NUCLEAR EQUATION OF STATE: OUTFLOW AND NEUTRINO-COOLED DISK FOR A LOW-MASS, HIGH-SPIN CASE” (2013, ApJ, 776, 47)","year":2016,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Neutron star; Astrophysics; Outflow; Neutrino; Equation of state; Spin (aerodynamics); Black hole (networking); Star (game theory); Nuclear physics","score_opus":0.010633630328255575,"score_gpt":0.27322447487638146,"score_spread":0.26259084454812587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2413936025","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00065285113,0.0011434479,0.0003041212,0.056010652,0.9294735,0.000019827296,0.0013066576,0.00022834828,0.010860697],"genre_scores_gemma":[0.020509118,0.008788772,0.0031089208,0.11122141,0.3708442,0.00008969352,0.0057482608,0.0011022424,0.47858733],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99874413,0.00010863773,0.0002973974,0.00019732122,0.0005296002,0.0001228756],"domain_scores_gemma":[0.9956072,0.0011600745,0.00052075216,0.000324502,0.0020422114,0.00034522673],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014034229,0.0023421259,0.0014085459,0.0022014545,0.0035929675,0.0031161932,0.002448803,0.0058320262,0.029661741],"category_scores_gemma":[0.015155497,0.00082716945,0.001340127,0.0015604635,0.0018164503,0.0030937127,0.0015137699,0.006138296,0.022565322],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000409282,0.000013269598,0.00014633682,0.000053437074,0.0000069064167,0.00042737002,0.00002716375,0.00006310451,0.00007518083,0.0010957484,0.9950749,0.0029755572],"study_design_scores_gemma":[0.000060383845,0.000043527707,0.0034250454,0.00027900658,0.00004607098,0.0011151375,0.00022618659,0.00042323524,0.00061557116,0.0046090456,0.9890904,0.00006647382],"about_ca_topic_score_codex":0.022090526,"about_ca_topic_score_gemma":0.034301188,"teacher_disagreement_score":0.029661741,"about_ca_system_score_codex":0.0030117405,"about_ca_system_score_gemma":0.0034431003,"threshold_uncertainty_score":0.09922844},"labels":[],"label_agreement":null},{"id":"W2415112740","doi":"10.3847/1538-4357/833/2/228","title":"Bicep2/KECK ARRAY VIII: MEASUREMENT OF GRAVITATIONAL LENSING FROM LARGE-SCALE B-MODE POLARIZATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; University of British Columbia; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Gravitational lens; Cosmic microwave background; Polarization (electrochemistry); Weak gravitational lensing; Cosmology; Angular resolution (graph drawing); Amplitude; Strong gravitational lensing; Angular diameter","score_opus":0.010881377854774452,"score_gpt":0.2416827396027091,"score_spread":0.23080136174793467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2415112740","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96709764,0.0002670746,0.006631707,0.00012494824,0.00003098558,0.000033499247,0.01111173,0.0003671761,0.014335086],"genre_scores_gemma":[0.9794124,0.00010470757,0.0081103025,0.000090709276,0.000033224576,0.00006562232,0.010903519,0.00010730836,0.0011721851],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99938476,0.00010111226,0.00002674021,0.00016966203,0.00018396665,0.00013380044],"domain_scores_gemma":[0.9988954,0.00017304074,0.00020123123,0.00026196588,0.00027914328,0.00018916548],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00085064635,0.00054610334,0.00029564774,0.0018415196,0.0004910586,0.0008796192,0.0005059369,0.00043001788,0.0030318275],"category_scores_gemma":[0.0015357176,0.0003810036,0.00029650444,0.0016322518,0.00030915253,0.0006292846,0.0014351276,0.0006525643,0.001047411],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019390911,0.00036443098,0.6709574,0.00026679382,0.0009846842,0.00092043384,0.00043691281,0.008490193,0.2450496,0.0049887593,0.013248207,0.05235346],"study_design_scores_gemma":[0.000040058818,0.000116464515,0.9473287,0.000030563184,0.00008390529,0.0005039534,0.00008150034,0.0067353346,0.038062755,0.0008131468,0.0061370176,0.00006661501],"about_ca_topic_score_codex":0.0025286842,"about_ca_topic_score_gemma":0.0041421405,"teacher_disagreement_score":0.0030318275,"about_ca_system_score_codex":0.00026116642,"about_ca_system_score_gemma":0.00026988925,"threshold_uncertainty_score":0.010142446},"labels":[],"label_agreement":null},{"id":"W2415297775","doi":"10.3847/0004-637x/827/1/58","title":"OBSCURED AGNs IN BULGELESS HOSTS DISCOVERED BY WISE: THE CASE STUDY OF SDSS J1224+5555","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supermassive black hole; Galaxy; Active galactic nucleus; Luminosity; Black hole (networking); Quasar; Intermediate-mass black hole","score_opus":0.007932276356645129,"score_gpt":0.22605332261184763,"score_spread":0.2181210462552025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2415297775","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994646,0.0000871066,0.00003169777,0.000040365223,0.0000027119875,0.000004876738,0.000055005494,0.000006106344,0.00030756707],"genre_scores_gemma":[0.999572,0.000055848403,0.000066579356,0.000033936598,0.00000853557,0.0000014754042,0.000073858944,0.000002208784,0.00018557392],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984896,0.000014837181,0.000013082944,0.000043097836,0.000028911598,0.000051050916],"domain_scores_gemma":[0.99969053,0.00002417839,0.00008977854,0.00002432043,0.000027067179,0.0001441656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019526205,0.00041997747,0.00022324579,0.001904575,0.0008068552,0.00056887785,0.00033769823,0.000372071,0.0010069102],"category_scores_gemma":[0.00045304748,0.00020431141,0.00018052771,0.00065945875,0.0005713906,0.00033058546,0.00093746546,0.0002976992,0.00020784147],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008934616,0.00005716393,0.9553495,0.000025478179,0.0000335927,0.0337292,0.001712615,0.000049280174,0.0034929833,0.0001108381,0.0005459926,0.0048039975],"study_design_scores_gemma":[0.000008263715,0.00013901693,0.9550451,0.000021680968,0.00004950778,0.03924442,0.00247246,0.00020296659,0.0010462597,0.00007235471,0.0016863815,0.000011606203],"about_ca_topic_score_codex":0.011219941,"about_ca_topic_score_gemma":0.02164477,"teacher_disagreement_score":0.011219941,"about_ca_system_score_codex":0.00043555873,"about_ca_system_score_gemma":0.00019840295,"threshold_uncertainty_score":0.022309303},"labels":[],"label_agreement":null},{"id":"W2415655701","doi":"10.3847/0004-637x/826/2/162","title":"THE IMPACT OF SURFACE TEMPERATURE INHOMOGENEITIES ON QUIESCENT NEUTRON STAR RADIUS MEASUREMENTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"RADIUS; Hot spot (computer programming); Neutron star; Spectral line; Globular cluster; Thermal; Range (aeronautics); Stars","score_opus":0.02161611237142524,"score_gpt":0.256193604525121,"score_spread":0.23457749215369578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2415655701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982686,0.000027701963,0.0011165814,0.00001190228,0.0000022328645,0.000003848192,0.000109542176,0.000056087516,0.00040353835],"genre_scores_gemma":[0.999355,0.0000067997867,0.00042298622,0.00000652403,6.622987e-7,0.0000024130604,0.00014199117,0.000013770889,0.00004982206],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996567,0.000085139065,0.000018954855,0.00011540878,0.00006283781,0.00006097307],"domain_scores_gemma":[0.99869305,0.0006826021,0.00017555911,0.00021493301,0.00014618029,0.000087628956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008792665,0.0003182701,0.00022491977,0.0002791348,0.00043060863,0.0006032668,0.0006690842,0.00033326066,0.00057637604],"category_scores_gemma":[0.0027035433,0.00022120391,0.00029247245,0.00039084037,0.00047805137,0.00037718637,0.000372599,0.00025119924,0.00009624162],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006940617,0.00009310287,0.6285788,0.00004626387,0.00019854955,0.00016450623,0.00024372827,0.3258269,0.034262136,0.00076489773,0.00023488449,0.008892054],"study_design_scores_gemma":[0.00007098185,0.00027854732,0.454973,0.000017522641,0.00012394623,0.00011005686,0.00019878469,0.5034103,0.03918707,0.00065745943,0.0009270546,0.000045310393],"about_ca_topic_score_codex":0.020261496,"about_ca_topic_score_gemma":0.014796239,"teacher_disagreement_score":0.020261496,"about_ca_system_score_codex":0.000815793,"about_ca_system_score_gemma":0.00034166407,"threshold_uncertainty_score":0.040287137},"labels":[],"label_agreement":null},{"id":"W2416147344","doi":"10.3847/0004-637x/827/1/42","title":"KOMPANEETS MODEL FITTING OF THE ORION–ERIDANUS SUPERBUBBLE. II. THINKING OUTSIDE OF BARNARD’S LOOP","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Superbubble; Astrophysics; Physics; Scale (ratio); Star (game theory); Astronomy; Interstellar medium; Galaxy","score_opus":0.013318362779786477,"score_gpt":0.22754935039626287,"score_spread":0.21423098761647638,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2416147344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9848155,0.00015839389,0.006609127,0.00037332863,0.00004410827,0.000034481298,0.00040980353,0.0002985191,0.0072567235],"genre_scores_gemma":[0.9962847,0.000038885646,0.0014818076,0.00009654607,0.000011597639,0.000019324394,0.00026831686,0.00012850258,0.0016702313],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99972504,0.000065326385,0.000012626592,0.000082114195,0.000056832916,0.000058016667],"domain_scores_gemma":[0.9992169,0.00028453962,0.000106181804,0.0000805646,0.00015494012,0.00015681075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060795137,0.0007006076,0.00084106845,0.00060591137,0.00095471623,0.0010895198,0.0018102833,0.0015751715,0.0028639815],"category_scores_gemma":[0.0021636002,0.00044332875,0.0008788568,0.0005146097,0.00045836074,0.0010893252,0.00066454004,0.0010519992,0.0006104678],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014690899,0.00010238466,0.01800706,0.000034833432,0.00008128117,0.00032161464,0.0001947968,0.9705631,0.0030698255,0.0028349727,0.0012339064,0.0034093708],"study_design_scores_gemma":[0.000053510328,0.000029010554,0.004899338,0.000006332364,0.000016332247,0.000047853497,0.00009008627,0.9926745,0.00048198193,0.0010092962,0.00067090883,0.000020795762],"about_ca_topic_score_codex":0.042307276,"about_ca_topic_score_gemma":0.02599869,"teacher_disagreement_score":0.042307276,"about_ca_system_score_codex":0.0015477623,"about_ca_system_score_gemma":0.00086448673,"threshold_uncertainty_score":0.08412206},"labels":[],"label_agreement":null},{"id":"W2416426348","doi":"10.3847/1538-4357/aa60c5","title":"The ISLAndS Project. II. The Lifetime Star Formation Histories of Six Andromeda dSphs*","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Ministerio de Economía y Competitividad; Jet Propulsion Laboratory; Space Telescope Science Institute; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Andromeda; Astronomy; Andromeda Galaxy; Star (game theory); Geography; History; Physics; Astrophysics; Milky Way; Galaxy","score_opus":0.01225240303393729,"score_gpt":0.23635859229858214,"score_spread":0.22410618926464485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2416426348","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9531728,0.0007986892,0.0009222084,0.00014651827,0.000011712695,0.00011521209,0.03349651,0.00024363035,0.0110925995],"genre_scores_gemma":[0.9234126,0.00045828012,0.006435168,0.000100210804,0.000027837144,0.00014888581,0.058229204,0.00019144794,0.010996337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998115,0.000036054975,0.000007906545,0.000054135202,0.000056675774,0.00003381574],"domain_scores_gemma":[0.99922574,0.00006945568,0.00014587853,0.00014197918,0.00015226753,0.00026469887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053192524,0.00034450387,0.00017745572,0.0009416277,0.00023240945,0.00045064042,0.00034332683,0.0001436504,0.0020371072],"category_scores_gemma":[0.00071262085,0.00014383708,0.00020868701,0.0005044133,0.00014528983,0.0003014159,0.0010840916,0.00022369089,0.0009941908],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016753591,0.00020261378,0.8296719,0.00025354297,0.00039810743,0.00048092855,0.002042517,0.0013621766,0.016702147,0.0018622958,0.017203327,0.12814504],"study_design_scores_gemma":[0.000054817916,0.00013992692,0.96606934,0.000030024137,0.000071216564,0.00025969197,0.00040506522,0.0006990311,0.0027338008,0.00022894601,0.02929153,0.000016632452],"about_ca_topic_score_codex":0.0355778,"about_ca_topic_score_gemma":0.062386867,"teacher_disagreement_score":0.0355778,"about_ca_system_score_codex":0.00053120556,"about_ca_system_score_gemma":0.00041042516,"threshold_uncertainty_score":0.070741415},"labels":[],"label_agreement":null},{"id":"W2418081591","doi":"10.3847/0004-637x/827/2/107","title":"MID-J CO SHOCK TRACING OBSERVATIONS OF INFRARED DARK CLOUDS. III. SLED FITTING","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; Western University","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Physics; Protostar; Line (geometry); Infrared; Photodissociation; Shock (circulatory); Emission spectrum; Spectral line; Molecular cloud; Star formation; Astronomy; Stars; Chemistry","score_opus":0.020905095842912245,"score_gpt":0.25289933181572527,"score_spread":0.23199423597281302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2418081591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98838484,0.00010284614,0.0073829186,0.00014679857,0.000018692914,0.000027745997,0.0010536592,0.0009337855,0.0019486621],"genre_scores_gemma":[0.9956476,0.000020590383,0.002609722,0.000043355598,0.0000052475207,0.000009390615,0.0010661902,0.00009849932,0.00049936614],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9997371,0.000046398178,0.00002141349,0.000090671245,0.00004900419,0.000055442924],"domain_scores_gemma":[0.9994697,0.00019550978,0.00006769885,0.00009224384,0.000103017184,0.000071883296],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007235035,0.0007059116,0.00045397587,0.0009842381,0.00042988575,0.00090803317,0.0007976552,0.00085015246,0.0010487379],"category_scores_gemma":[0.0016102361,0.0003293181,0.0009830802,0.0005586841,0.0002229767,0.00038520407,0.0004842987,0.00065891753,0.0004622201],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005252419,0.00018853527,0.15960138,0.00005821477,0.00020927725,0.00023967618,0.00012957334,0.81106746,0.008432383,0.0006843172,0.0013285889,0.017535344],"study_design_scores_gemma":[0.000026165731,0.00003289225,0.02896003,0.0000048753127,0.000012960365,0.000025857882,0.000048550624,0.96869713,0.0016101182,0.0002801879,0.00028700693,0.0000143100715],"about_ca_topic_score_codex":0.012765225,"about_ca_topic_score_gemma":0.009541326,"teacher_disagreement_score":0.012765225,"about_ca_system_score_codex":0.0009335125,"about_ca_system_score_gemma":0.00032543027,"threshold_uncertainty_score":0.025381863},"labels":[],"label_agreement":null},{"id":"W2434822230","doi":"10.3847/1538-4357/aa7206","title":"A Spectroscopic Follow-up Program of Very Massive Galaxies at 3 &lt; z &lt; 4: Confirmation of Spectroscopic Redshifts, and a High Fraction of Powerful AGNs","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Photometry (optics); Galaxy; Redshift; Active galactic nucleus; COSMIC cancer database; Emission spectrum; Luminous infrared galaxy; Spectral line; Stellar mass","score_opus":0.007678978457388779,"score_gpt":0.23779168348532095,"score_spread":0.23011270502793219,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2434822230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937004,0.000018856885,0.0001278528,0.000017636914,0.000001215466,0.000012135125,0.000263435,0.000013300643,0.00017557477],"genre_scores_gemma":[0.99888414,0.00001081112,0.00027215166,0.000013599085,0.0000033233252,0.0000097368065,0.00049686397,0.0000029899104,0.00030635975],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996729,0.00005871417,0.000019803612,0.00006434791,0.0000832476,0.00010093318],"domain_scores_gemma":[0.99817145,0.00020284079,0.00049403426,0.00017610595,0.0004248578,0.00053075684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006570359,0.00023796973,0.0002287528,0.0016867387,0.00052980083,0.00043879074,0.00039251745,0.00031743554,0.0010549579],"category_scores_gemma":[0.0011861235,0.00013786218,0.00027220754,0.0006034479,0.00018482562,0.00029613182,0.00061372714,0.00028447047,0.0004748943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000063240856,0.00006484797,0.9922814,0.000004551153,0.000010344472,0.00010883962,0.00015299465,0.00006303216,0.004453048,0.000012882243,0.00010117132,0.0026837047],"study_design_scores_gemma":[0.0000025424074,0.000057227713,0.99850816,9.92821e-7,0.0000074551613,0.00007135021,0.0000716829,0.00023950517,0.00089142355,0.0000051381116,0.00014281321,0.0000016357336],"about_ca_topic_score_codex":0.013544694,"about_ca_topic_score_gemma":0.013758844,"teacher_disagreement_score":0.013544694,"about_ca_system_score_codex":0.00038382105,"about_ca_system_score_gemma":0.00029628683,"threshold_uncertainty_score":0.026931703},"labels":[],"label_agreement":null},{"id":"W2436180047","doi":"10.3847/1538-4357/833/1/72","title":"ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: THE INFRARED EXCESS OF UV-SELECTED z = 2–10 GALAXIES AS A FUNCTION OF UV-CONTINUUM SLOPE AND STELLAR MASS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":274,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Deutsche Forschungsgemeinschaft; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Galaxy; Redshift; Infrared; Stellar mass; Luminous infrared galaxy; Luminosity; Hubble Ultra-Deep Field","score_opus":0.007260212404988143,"score_gpt":0.20791773816098388,"score_spread":0.20065752575599574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2436180047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992206,0.00004524223,0.000042689342,0.00001457121,0.0000013698722,0.0000015551178,0.0003100228,0.000009024979,0.00035481516],"genre_scores_gemma":[0.99899405,0.0000297939,0.000081438826,0.00001946806,0.000006152929,0.0000027959686,0.0005972629,0.0000022244515,0.00026674106],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979967,0.000037265407,0.0000100657235,0.000058475838,0.0000408203,0.000053836673],"domain_scores_gemma":[0.99859565,0.00019325978,0.00048025468,0.00010980214,0.00014702934,0.00047401196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004746135,0.00027187375,0.0002276388,0.002075568,0.00021797215,0.0004933331,0.00028511725,0.0002787452,0.001437706],"category_scores_gemma":[0.0009405683,0.00015556869,0.00016793273,0.00056606636,0.00022777278,0.00034326775,0.00042727287,0.00022595623,0.0004188117],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057091722,0.000024720825,0.9959578,0.000004763584,0.000021127606,0.00003428891,0.00007292296,0.00003130401,0.0021865948,0.000025983187,0.00011568128,0.0014677149],"study_design_scores_gemma":[0.0000010443489,0.000010736429,0.9997167,0.0000012035985,0.000002914966,0.000030799325,0.000025636626,0.000055091514,0.00009046875,0.000004251727,0.000060487553,6.778595e-7],"about_ca_topic_score_codex":0.005236946,"about_ca_topic_score_gemma":0.009952098,"teacher_disagreement_score":0.005236946,"about_ca_system_score_codex":0.0002392818,"about_ca_system_score_gemma":0.000084888634,"threshold_uncertainty_score":0.010412931},"labels":[],"label_agreement":null},{"id":"W2461463152","doi":"10.3847/1538-4357/833/2/244","title":"NEUTRON STAR MASS–RADIUS CONSTRAINTS USING EVOLUTIONARY OPTIMIZATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; University of Calgary; University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Leids Kerkhoven-Bosscha Fonds","keywords":"Physics; Neutron star; RADIUS; Astrophysics; Neutron; Equation of state; Computational physics; Thermonuclear fusion; Parameter space; Nuclear physics; Statistics; Mathematics; Computer science","score_opus":0.015725350721103978,"score_gpt":0.2976964634816077,"score_spread":0.28197111276050374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2461463152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.55803806,0.00034242633,0.42996663,0.00044302762,0.000032121243,0.000095029165,0.00030708924,0.0005126911,0.010262964],"genre_scores_gemma":[0.9173666,0.000066469045,0.08078289,0.00009787971,0.000018689063,0.00007143558,0.0003590255,0.00013236572,0.0011045883],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99965096,0.00015609701,0.000016132113,0.00007522724,0.0000612457,0.000040426457],"domain_scores_gemma":[0.9984158,0.0010094113,0.00018459192,0.00011451914,0.00020718611,0.00006845845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014764336,0.0007068575,0.00084958033,0.000965651,0.0005452631,0.00093023636,0.00084683596,0.001070822,0.0011874954],"category_scores_gemma":[0.0064009908,0.00054904755,0.0005911542,0.0005847118,0.0006046869,0.0006826473,0.0006067473,0.0006586588,0.00024307406],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000017821147,0.000013781507,0.0011393348,0.000006804828,0.000011276224,0.000017060609,0.000011196221,0.99367684,0.00046833445,0.001385771,0.00010003114,0.0031517015],"study_design_scores_gemma":[0.0000034878199,0.000004770013,0.00019927428,0.0000020730022,0.0000012089744,0.0000037129064,0.0000024363587,0.9989925,0.00014113894,0.0005795152,0.000067944195,0.0000019262877],"about_ca_topic_score_codex":0.0073060454,"about_ca_topic_score_gemma":0.0039499947,"teacher_disagreement_score":0.0073060454,"about_ca_system_score_codex":0.0010287542,"about_ca_system_score_gemma":0.00091730914,"threshold_uncertainty_score":0.014527023},"labels":[],"label_agreement":null},{"id":"W2461817708","doi":"10.3847/0004-637x/824/2/150","title":"A COMBINED SPECTROSCOPIC AND PHOTOMETRIC STELLAR ACTIVITY STUDY OF EPSILON ERIDANI","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Cape Breton University; University of British Columbia","funders":"","keywords":"Photometry (optics); Stars; Stellar atmosphere; Young stellar object; Radial velocity; Astronomical spectroscopy; Spectral line; Starspot","score_opus":0.012250540004233017,"score_gpt":0.2381683417653354,"score_spread":0.2259178017611024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2461817708","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99863213,0.000022530017,0.00020359426,0.0000076776405,0.0000013021944,0.0000024688459,0.00009657662,0.0000067502638,0.0010270376],"genre_scores_gemma":[0.9982516,0.00003321175,0.0007235418,0.000013459683,0.0000022037468,0.0000029250862,0.00028735894,0.000008836812,0.00067678833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980885,0.000017310445,0.000009655694,0.000083182334,0.000047895643,0.000033117736],"domain_scores_gemma":[0.9996327,0.000059218357,0.00008840592,0.00005371712,0.00011020986,0.000055691013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039779514,0.00036795664,0.0002728842,0.00087864464,0.000333383,0.0003650495,0.00046160232,0.00020700313,0.00049972197],"category_scores_gemma":[0.0004055854,0.00015973911,0.00018976862,0.00041508465,0.00021132083,0.00031068455,0.00055656716,0.00022101628,0.000287648],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030321235,0.00016617184,0.92581767,0.00003608465,0.00007033408,0.0008194657,0.0008990077,0.001951329,0.035851005,0.00030805773,0.00035388916,0.03342368],"study_design_scores_gemma":[0.0000074532995,0.00010750601,0.9904544,0.000009141993,0.000018779023,0.00030858602,0.00032877486,0.0028849505,0.0046313605,0.000075446056,0.0011642666,0.000009241398],"about_ca_topic_score_codex":0.009301076,"about_ca_topic_score_gemma":0.01691811,"teacher_disagreement_score":0.009301076,"about_ca_system_score_codex":0.00054342614,"about_ca_system_score_gemma":0.00019099937,"threshold_uncertainty_score":0.018493831},"labels":[],"label_agreement":null},{"id":"W2462963816","doi":"10.3847/1538-4357/834/2/133","title":"A COUPLED 2 × 2D BABCOCK–LEIGHTON SOLAR DYNAMO MODEL. II. REFERENCE DYNAMO SOLUTIONS","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Collège de Bois-de-Boulogne","funders":"","keywords":"Dynamo; Solar dynamo; Amplitude; Rotational symmetry; Solar cycle; Magnetic flux; Dipole; Magnetic field; Meridional flow","score_opus":0.02075494670314437,"score_gpt":0.25382445795223124,"score_spread":0.23306951124908687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2462963816","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8052615,0.0005650623,0.15047848,0.0009824903,0.00014941343,0.00013374367,0.00071142556,0.0002843444,0.04143364],"genre_scores_gemma":[0.98127395,0.00013762634,0.01176115,0.000113809234,0.00003607096,0.00016112645,0.00025260734,0.000049584665,0.0062140636],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999162,0.000027251248,0.000003916715,0.000021306378,0.000017636508,0.000013625682],"domain_scores_gemma":[0.999795,0.00006831703,0.000041061012,0.000021094993,0.000038343325,0.000036105408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002563017,0.0004151163,0.00072394003,0.00036067358,0.00044907353,0.0009827688,0.0011005182,0.0015150943,0.002450081],"category_scores_gemma":[0.00093113905,0.00033294025,0.0007096393,0.00032326233,0.0007318451,0.0006368925,0.00071338937,0.0005636909,0.00020023939],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003181707,0.000014515952,0.0006208556,0.000013502139,0.000020482334,0.000081800055,0.000027775888,0.9873815,0.0007706928,0.009799704,0.0002133185,0.0010239444],"study_design_scores_gemma":[0.000015790076,0.000009482176,0.00018987193,0.0000014684916,0.0000034704792,0.000008977433,0.0000071045456,0.99766123,0.00005859518,0.0018444107,0.00019517074,0.00000439419],"about_ca_topic_score_codex":0.011782695,"about_ca_topic_score_gemma":0.0038911744,"teacher_disagreement_score":0.011782695,"about_ca_system_score_codex":0.00083588995,"about_ca_system_score_gemma":0.00057870697,"threshold_uncertainty_score":0.023428261},"labels":[],"label_agreement":null},{"id":"W2464783573","doi":"10.3847/0004-637x/830/2/127","title":"CARMA LARGE AREA STAR FORMATION SURVEY: DENSE GAS IN THE YOUNG L1451 REGION OF PERSEUS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Serpens; Star formation; Molecular cloud; Hydrostatic equilibrium; Supersonic speed; Virial theorem; Young stellar object","score_opus":0.021646418468118392,"score_gpt":0.24219867300901596,"score_spread":0.22055225454089755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2464783573","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979013,0.000095416915,0.00004977085,0.00003248915,0.000002004075,0.0000085027705,0.001006838,0.000021749785,0.0008818557],"genre_scores_gemma":[0.99776185,0.000066837674,0.0002184491,0.00002969048,0.000006358028,0.000007144168,0.0013545387,0.000005077611,0.0005501067],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999455,0.0000062493477,0.0000026863556,0.000018810899,0.000014000913,0.0000127305175],"domain_scores_gemma":[0.99980456,0.000012976608,0.000052697746,0.0000129747505,0.000032852724,0.00008390117],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000103968465,0.00014932394,0.000111796486,0.0010411062,0.00024093353,0.0002931106,0.00018955306,0.000108624154,0.0014700853],"category_scores_gemma":[0.0001897648,0.00006403197,0.00008371968,0.00042872943,0.00011691265,0.000149586,0.00036395318,0.00009810856,0.00033816072],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010740235,0.000060778828,0.9734036,0.0000328057,0.000029650653,0.00038024026,0.00087169604,0.00023903293,0.009514388,0.000113910966,0.001902596,0.013343972],"study_design_scores_gemma":[0.000004757267,0.00002036005,0.9978598,0.0000030545625,0.0000036520657,0.000071352384,0.000194733,0.00012495473,0.00036631408,0.000011833201,0.0013374374,0.0000018423644],"about_ca_topic_score_codex":0.043284044,"about_ca_topic_score_gemma":0.070367515,"teacher_disagreement_score":0.043284044,"about_ca_system_score_codex":0.0004913754,"about_ca_system_score_gemma":0.00024004294,"threshold_uncertainty_score":0.08606422},"labels":[],"label_agreement":null},{"id":"W2465266626","doi":"10.3847/0004-637x/827/1/8","title":"FRIENDS OF HOT JUPITERS. IV. STELLAR COMPANIONS BEYOND 50 au MIGHT FACILITATE GIANT PLANET FORMATION, BUT MOST ARE UNLIKELY TO CAUSE KOZAI–LIDOV MIGRATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":139,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Hot Jupiter; Giant planet; Planetary system; Planet; Gas giant; Population; Stellar evolution; Stellar mass; Stars","score_opus":0.016934791688133884,"score_gpt":0.21855773140967102,"score_spread":0.20162293972153714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2465266626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99842,0.00011697527,0.00007141212,0.000032289205,0.0000042335682,0.000002138227,0.00009574789,0.000007016749,0.0012502155],"genre_scores_gemma":[0.9992803,0.000023562472,0.000053966218,0.000009646908,0.0000048662882,9.344805e-7,0.000095269985,0.0000011498516,0.00053033116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998784,0.000013018347,0.0000063553302,0.00004062068,0.000020983864,0.000040623658],"domain_scores_gemma":[0.9989838,0.0001491828,0.00045814968,0.00007949263,0.000057625115,0.00027167803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012955978,0.00009390552,0.00015435337,0.0007196417,0.00074880465,0.00045684646,0.00017877175,0.00019882715,0.0061049205],"category_scores_gemma":[0.00093891635,0.00008583572,0.00010624686,0.00039135225,0.00029062957,0.00033282503,0.00045964448,0.00018480976,0.00059861515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001108372,0.000017515064,0.9844482,0.000022635693,0.000037162903,0.0003133502,0.0004436895,0.00005757797,0.006037821,0.00024540268,0.00033042702,0.0079353135],"study_design_scores_gemma":[0.0000026262294,0.00003711811,0.9965527,0.0000042357738,0.000011415319,0.00062844256,0.00047291932,0.0001309439,0.0007999865,0.00008931284,0.001268254,0.000001950498],"about_ca_topic_score_codex":0.0017302774,"about_ca_topic_score_gemma":0.0028054125,"teacher_disagreement_score":0.0061049205,"about_ca_system_score_codex":0.0002123238,"about_ca_system_score_gemma":0.00010998339,"threshold_uncertainty_score":0.020422995},"labels":[],"label_agreement":null},{"id":"W2467984654","doi":"10.3847/0004-637x/830/2/62","title":"THE DRAGONFLY NEARBY GALAXIES SURVEY. I. SUBSTANTIAL VARIATION IN THE DIFFUSE STELLAR HALOS AROUND SPIRAL GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Spiral galaxy; Halo; Galaxy; Luminous infrared galaxy; Stellar mass; Disc; Galactic halo; Elliptical galaxy; Surface brightness","score_opus":0.012089956269185374,"score_gpt":0.21806430895543727,"score_spread":0.2059743526862519,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2467984654","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99839056,0.000061540966,0.000033523407,0.000014636035,0.0000010671766,0.0000021501344,0.000956077,0.0000066516486,0.00053382275],"genre_scores_gemma":[0.9973882,0.000039029415,0.00012468694,0.000011847206,0.0000026688888,0.000002559442,0.0021332186,0.0000024710484,0.0002954997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998579,0.000018229299,0.000007677291,0.00005753035,0.000028873474,0.000029826546],"domain_scores_gemma":[0.99953616,0.00007598443,0.00014620343,0.00005868151,0.000056064124,0.00012693339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019856798,0.00018229724,0.00013689073,0.0013363837,0.00028625768,0.0003884849,0.0001702465,0.00017327776,0.00077071873],"category_scores_gemma":[0.0004964129,0.00011181472,0.00012614684,0.00078506867,0.00025905573,0.00023248127,0.00033216254,0.00009054525,0.00017935396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059207254,0.000006567044,0.9928826,0.000010160629,0.000030994895,0.000039035018,0.00019523354,0.00009454582,0.0023766393,0.000041046766,0.00036753505,0.0038964723],"study_design_scores_gemma":[0.0000011246667,0.00000576001,0.99945194,0.0000018005612,0.000003369147,0.000025728257,0.00005923538,0.000054617514,0.0001031884,0.000003618792,0.0002888534,8.6538654e-7],"about_ca_topic_score_codex":0.027374707,"about_ca_topic_score_gemma":0.10262914,"teacher_disagreement_score":0.027374707,"about_ca_system_score_codex":0.00047233704,"about_ca_system_score_gemma":0.00013203027,"threshold_uncertainty_score":0.054430723},"labels":[],"label_agreement":null},{"id":"W2470433392","doi":"10.3847/0004-637x/830/2/135","title":"VELOCITY VARIATIONS IN THE PHOENIX–HERMUS STAR STREAM","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Dark matter; Halo; Milky Way; Globular cluster; RADIUS; Galaxy; Dark matter halo; Stars; Astronomy","score_opus":0.00813272847506292,"score_gpt":0.21219079789450046,"score_spread":0.20405806941943755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2470433392","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99897313,0.0000131981615,0.0003531316,0.000027940348,0.0000027038946,0.0000043222703,0.00009869909,0.0000150710775,0.00051189057],"genre_scores_gemma":[0.9992052,0.000015930176,0.0003120829,0.000006287598,0.0000016041947,0.000002276125,0.00014775152,0.000005211086,0.00030391707],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999572,0.000007042084,0.0000021133685,0.000011660167,0.000008340763,0.000013581625],"domain_scores_gemma":[0.99974424,0.000062339874,0.000041761825,0.000027088594,0.000046602152,0.00007797717],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029100277,0.00016358492,0.00018911003,0.00034013804,0.00036248585,0.00059700356,0.00031717448,0.0002534904,0.0010572905],"category_scores_gemma":[0.00086453,0.00015620397,0.00018129843,0.0002938585,0.00038656962,0.000400328,0.00040585807,0.00028755862,0.00015908049],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071539555,0.00032650933,0.42729503,0.00004817763,0.00022150912,0.0008843582,0.0004047171,0.53360397,0.014217212,0.0068489374,0.0026614084,0.012772829],"study_design_scores_gemma":[0.00014533376,0.00023616716,0.13372517,0.000011243452,0.000039476374,0.00009365197,0.00025103017,0.8568138,0.005154716,0.001887469,0.0016135157,0.000028475557],"about_ca_topic_score_codex":0.012183339,"about_ca_topic_score_gemma":0.008184174,"teacher_disagreement_score":0.012183339,"about_ca_system_score_codex":0.00072755414,"about_ca_system_score_gemma":0.00030404114,"threshold_uncertainty_score":0.024224818},"labels":[],"label_agreement":null},{"id":"W2471197113","doi":"10.3847/0004-637x/829/1/4","title":"THE BINARY BLACK HOLE MODEL FOR MRK 231 BITES THE DUST","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Quasar; Spectral energy distribution; Infrared; Galaxy; Astronomy; Spectral line; Binary number; Thermal; Emission spectrum","score_opus":0.020616600841789415,"score_gpt":0.24342416058410138,"score_spread":0.22280755974231198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2471197113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9719507,0.00020991889,0.0085491575,0.0017050009,0.00007083867,0.000036509166,0.00013857111,0.00008330549,0.017256074],"genre_scores_gemma":[0.99672276,0.000034406345,0.00051876483,0.000060258455,0.000022734852,0.000005313104,0.000024682615,0.0000070084698,0.0026041537],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998839,0.000022822927,0.0000056402587,0.00002814699,0.000019997347,0.000039554667],"domain_scores_gemma":[0.9996166,0.000053702835,0.00010098305,0.00004382755,0.000021853302,0.00016312618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004675272,0.00050690596,0.00056822755,0.00057561154,0.000904352,0.0017519005,0.001168935,0.0012485036,0.0063292338],"category_scores_gemma":[0.0005982881,0.00020319202,0.0006036297,0.00022933347,0.0012128911,0.001109213,0.0010825369,0.00063176284,0.0009973443],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001094794,0.00077856396,0.09699894,0.00013493405,0.00017250133,0.013444709,0.0013467526,0.07028821,0.022676084,0.7716931,0.005947679,0.015423765],"study_design_scores_gemma":[0.00069258636,0.0007613061,0.04313826,0.000056751112,0.00017195354,0.006947552,0.001109943,0.65481436,0.0019131149,0.2832656,0.007004647,0.00012397699],"about_ca_topic_score_codex":0.0029793468,"about_ca_topic_score_gemma":0.0017402337,"teacher_disagreement_score":0.0063292338,"about_ca_system_score_codex":0.0005843524,"about_ca_system_score_gemma":0.00034263593,"threshold_uncertainty_score":0.021173418},"labels":[],"label_agreement":null},{"id":"W2473931356","doi":"10.3847/0004-637x/831/1/16","title":"A PORTRAIT OF COLD GAS IN GALAXIES AT 60 pc RESOLUTION AND A SIMPLE METHOD TO TEST HYPOTHESES THAT LINK SMALL-SCALE ISM STRUCTURE TO GALAXY-SCALE PROCESSES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":112,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Institutes of Natural Sciences; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; National Science Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; European Commission; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Galaxy; Line (geometry); Interstellar medium; Scaling; Gravitational potential; Molecular cloud; Star formation; Log-normal distribution; Angular resolution (graph drawing)","score_opus":0.01548586948167913,"score_gpt":0.24842696721598864,"score_spread":0.23294109773430952,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2473931356","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9896836,0.00017167206,0.006856828,0.000052365158,0.0000030466401,0.000003693938,0.0002637726,0.00013556879,0.0028293896],"genre_scores_gemma":[0.99803907,0.000036410554,0.0016015169,0.000014133699,0.000004083071,0.0000024062817,0.00015206756,0.000011537867,0.00013885778],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993956,0.000008270247,0.0000024858184,0.000016983113,0.000017338583,0.00001535873],"domain_scores_gemma":[0.99973553,0.000092988055,0.000043545857,0.000038851013,0.00003531829,0.00005388628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013420575,0.00010421115,0.00014905664,0.0011867202,0.00019443512,0.00034073245,0.00017191873,0.00015379759,0.0014061381],"category_scores_gemma":[0.0003990858,0.00009072883,0.00017723792,0.00058623543,0.00022879182,0.00024536808,0.0002661988,0.0002082374,0.00021898244],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035636095,0.0001348602,0.5972556,0.00010897228,0.00017831827,0.0008265945,0.0011330312,0.021800233,0.319202,0.007819176,0.0013891181,0.049795672],"study_design_scores_gemma":[0.0000072519288,0.00005298104,0.95333064,0.0000103252705,0.00002446726,0.0004333849,0.00029173106,0.03088103,0.011971557,0.0016204662,0.001364473,0.000011715562],"about_ca_topic_score_codex":0.0027858699,"about_ca_topic_score_gemma":0.0025195696,"teacher_disagreement_score":0.0027858699,"about_ca_system_score_codex":0.00018906045,"about_ca_system_score_gemma":0.000051536197,"threshold_uncertainty_score":0.005539298},"labels":[],"label_agreement":null},{"id":"W2474039259","doi":"10.3847/0004-637x/831/1/17","title":"DETECTION OF SOLAR-LIKE OSCILLATIONS, OBSERVATIONAL CONSTRAINTS, AND STELLAR MODELS FOR θ CYG, THE BRIGHTEST STAR OBSERVED BY THE KEPLER MISSION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Asteroseismology; RADIUS; Amplitude; Angular diameter; Star (game theory); Oscillation (cell signaling); Stars; Stellar evolution; Red giant","score_opus":0.040758119805694736,"score_gpt":0.2350828668965166,"score_spread":0.19432474709082187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2474039259","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99788636,0.000047478286,0.00026857958,0.00003672261,0.0000015453012,0.000004719539,0.0006978603,0.00002040359,0.0010363344],"genre_scores_gemma":[0.9982318,0.0000263769,0.00038921944,0.000009054513,0.000003454476,0.0000027812,0.0012071597,0.000012306165,0.000117766336],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988425,0.000021233405,0.000007710999,0.000037229234,0.000024028452,0.000025478821],"domain_scores_gemma":[0.99943036,0.00013724079,0.00017671107,0.000060320417,0.000058571535,0.00013669766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044955857,0.00026826176,0.00021774924,0.000784111,0.00038482642,0.0005315978,0.00026215884,0.0002307704,0.0014419483],"category_scores_gemma":[0.0011648695,0.00017039574,0.00020039256,0.00047051752,0.00019404119,0.0003259463,0.00031339438,0.00027553985,0.00030424935],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010064293,0.000033005355,0.9877007,0.000009433152,0.000021796865,0.000102071084,0.00012071176,0.003561048,0.004894987,0.000278973,0.00056407007,0.0026126408],"study_design_scores_gemma":[0.0000094735515,0.000029955065,0.9883152,0.0000060016378,0.0000108198365,0.00007624131,0.00011421025,0.010141596,0.0005805217,0.00012507182,0.0005848058,0.0000060427415],"about_ca_topic_score_codex":0.01879261,"about_ca_topic_score_gemma":0.03409547,"teacher_disagreement_score":0.01879261,"about_ca_system_score_codex":0.0007286217,"about_ca_system_score_gemma":0.0003441955,"threshold_uncertainty_score":0.03736645},"labels":[],"label_agreement":null},{"id":"W2475009629","doi":"10.3847/0004-637x/825/2/134","title":"XMM-NEWTON AND CHANDRA OBSERVATIONS OF THE FILLED-CENTER SUPERNOVA REMNANT G63.7+1.1","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Pulsar wind nebula; Supernova remnant; Neutron star; Pulsar; Nebula; ROSAT; Supernova; Astronomy; Luminosity; Observatory; Galaxy; Stars","score_opus":0.021385105521441117,"score_gpt":0.28799170946775554,"score_spread":0.2666066039463144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2475009629","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747145,0.0003478104,0.00019505099,0.000036007383,0.00000681733,0.000011227171,0.00081335526,0.000059662925,0.0010585929],"genre_scores_gemma":[0.99390817,0.00019297069,0.0019290603,0.000057785248,0.000023011089,0.000016639866,0.002814777,0.000037438487,0.0010201201],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993,0.000006011302,0.000004048368,0.000020611784,0.000022003953,0.000017198403],"domain_scores_gemma":[0.99967384,0.000031125757,0.00010761663,0.000034812118,0.000052436302,0.00010021649],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027045852,0.0003294409,0.00032008794,0.001348375,0.00041714494,0.000318288,0.00030716648,0.0003159347,0.0011131406],"category_scores_gemma":[0.00020325849,0.00020246486,0.0003617047,0.00050745707,0.00016027203,0.00017507005,0.00047757517,0.00028229287,0.0004467849],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011804724,0.00029628872,0.47028077,0.00020590889,0.00027850852,0.0043289196,0.00090787985,0.00081955525,0.48807037,0.00058558263,0.0018754154,0.031170394],"study_design_scores_gemma":[0.000011602356,0.000071283546,0.9940263,0.0000069952575,0.000020602602,0.00064776343,0.00004188805,0.0004288764,0.0032723907,0.000039380822,0.0014275627,0.0000053679632],"about_ca_topic_score_codex":0.001395636,"about_ca_topic_score_gemma":0.003015689,"teacher_disagreement_score":0.001395636,"about_ca_system_score_codex":0.00019671611,"about_ca_system_score_gemma":0.00007002305,"threshold_uncertainty_score":0.0037238598},"labels":[],"label_agreement":null},{"id":"W2476819508","doi":"10.3847/1538-4357/833/1/69","title":"ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: CO LUMINOSITY FUNCTIONS AND THE EVOLUTION OF THE COSMIC DENSITY OF MOLECULAR GAS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Deutsche Forschungsgemeinschaft; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Redshift; Galaxy; COSMIC cancer database; Luminosity function; Star formation; Luminosity; Hubble Ultra-Deep Field; Physical cosmology","score_opus":0.005984000022363938,"score_gpt":0.20411371848804213,"score_spread":0.1981297184656782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2476819508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981998,0.00010917171,0.00033038954,0.000023459303,0.0000022153206,0.0000015820365,0.0006475626,0.000019379477,0.0006664127],"genre_scores_gemma":[0.9990381,0.000030032192,0.00019460464,0.00001031054,0.0000048147194,0.0000012834471,0.00056240783,0.0000029210773,0.00015570241],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998272,0.00004857878,0.000006446223,0.0000493435,0.00003373163,0.000034754758],"domain_scores_gemma":[0.99816763,0.00035954238,0.000744891,0.00019047751,0.00017505273,0.00036239668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005406402,0.0002137958,0.00019021753,0.00213332,0.00020207703,0.00056813005,0.00022247064,0.00021020854,0.0008782052],"category_scores_gemma":[0.0011694138,0.000100848156,0.00018577192,0.0011385856,0.00024810657,0.00041766439,0.00038824242,0.00018255433,0.0001946618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000084779815,0.000026120584,0.991343,0.000008583838,0.000055569268,0.000037894515,0.0000595084,0.0005950179,0.0031243723,0.0002580503,0.00019045029,0.004216477],"study_design_scores_gemma":[0.0000012251371,0.000008761854,0.99874437,0.0000015965152,0.0000062073877,0.00002108181,0.000015210748,0.00065873034,0.00033209944,0.00004475474,0.00016436086,0.0000015675287],"about_ca_topic_score_codex":0.007464161,"about_ca_topic_score_gemma":0.011025008,"teacher_disagreement_score":0.007464161,"about_ca_system_score_codex":0.00038783182,"about_ca_system_score_gemma":0.00012230397,"threshold_uncertainty_score":0.014841437},"labels":[],"label_agreement":null},{"id":"W2478284440","doi":"10.3847/0004-637x/830/1/38","title":"LOW-FREQUENCY OBSERVATIONS OF LINEARLY POLARIZED STRUCTURES IN THE INTERSTELLAR MEDIUM NEAR THE SOUTH GALACTIC POLE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Faraday effect; Polarization (electrochemistry); Linear polarization; Polarimetry; Optics; Astrophysics; Wavelength; Interstellar medium; Astronomical interferometer; Faraday cage; Polarimeter; Magnetic field; Interferometry; Galaxy","score_opus":0.014217011721791543,"score_gpt":0.22610105069197403,"score_spread":0.2118840389701825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2478284440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99818736,0.0001398029,0.00038024408,0.000040336832,0.0000048605534,0.0000021725136,0.00018846511,0.000021394615,0.0010354057],"genre_scores_gemma":[0.9987318,0.00007637018,0.0005917915,0.000018064962,0.000013930211,0.0000035042112,0.00033334547,0.0000040869654,0.00022716928],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995816,0.00000489736,0.0000012025258,0.000010438847,0.000013342935,0.0000119104125],"domain_scores_gemma":[0.9998554,0.000029790737,0.000039893504,0.000013302294,0.000024848898,0.000036822836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008178975,0.00017975202,0.00017474133,0.0007788642,0.0002802182,0.00030612544,0.00021407586,0.00018238765,0.0009752631],"category_scores_gemma":[0.00028770397,0.00016434459,0.00008081105,0.00038136932,0.00020677941,0.00026519413,0.00040453605,0.0002545563,0.00021252714],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036580788,0.000094731084,0.4725822,0.00008574195,0.00011885566,0.00061594124,0.0006025504,0.0017342789,0.49275708,0.0004750048,0.0012842205,0.029283574],"study_design_scores_gemma":[0.000029007231,0.000077185345,0.9914483,0.000010051837,0.000028365615,0.00017502543,0.00019262698,0.0015017729,0.0046869735,0.00019976508,0.0016401338,0.00001081078],"about_ca_topic_score_codex":0.0017041878,"about_ca_topic_score_gemma":0.006054663,"teacher_disagreement_score":0.0017041878,"about_ca_system_score_codex":0.00018755728,"about_ca_system_score_gemma":0.00006796985,"threshold_uncertainty_score":0.0033885837},"labels":[],"label_agreement":null},{"id":"W2478797237","doi":"10.3847/1538-4357/833/1/70","title":"THE ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: MOLECULAR GAS RESERVOIRS IN HIGH-REDSHIFT GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":124,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Deutsche Forschungsgemeinschaft; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Galaxy; Redshift; Hubble Ultra-Deep Field; Star formation; Infrared; Luminous infrared galaxy; Stellar mass; Context (archaeology); Hubble Deep Field; Astronomy","score_opus":0.007903233535472322,"score_gpt":0.2214326604158315,"score_spread":0.2135294268803592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2478797237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994646,0.000055339395,0.000058858055,0.000017374814,6.8811636e-7,0.0000010923615,0.00021040504,0.0000062799227,0.00018534035],"genre_scores_gemma":[0.9996057,0.000021643627,0.000061204155,0.0000066093044,0.0000036007305,0.0000011929702,0.00021901858,0.0000010161422,0.00007990433],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982834,0.00003638723,0.000007976895,0.000047296056,0.000031144435,0.0000488982],"domain_scores_gemma":[0.99881893,0.00018596719,0.00050516427,0.0001019298,0.00012964143,0.00025831844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038706782,0.00018300292,0.000214702,0.0017442004,0.000276488,0.00062355644,0.000312741,0.00028485424,0.0009738314],"category_scores_gemma":[0.00087180786,0.00010727456,0.00017082668,0.0012371601,0.00024709126,0.0006218525,0.00040688016,0.00016467871,0.0002141224],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034966735,0.000019634437,0.995861,0.000005141496,0.000015207114,0.000025792053,0.00008213677,0.00011609939,0.0017602001,0.00007334479,0.00009752765,0.0019089225],"study_design_scores_gemma":[0.0000010301684,0.000007938277,0.99945694,0.000001023522,0.0000032825003,0.00001588662,0.00004190272,0.0002468469,0.000110927904,0.000013555103,0.00009963077,0.0000010146703],"about_ca_topic_score_codex":0.010168851,"about_ca_topic_score_gemma":0.013965341,"teacher_disagreement_score":0.010168851,"about_ca_system_score_codex":0.00039050967,"about_ca_system_score_gemma":0.00013946815,"threshold_uncertainty_score":0.020219326},"labels":[],"label_agreement":null},{"id":"W2479368785","doi":"10.3847/0004-637x/830/2/104","title":"THE EXTREME ULTRAVIOLET VARIABILITY OF QUASARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Quasar; Rest frame; Extreme ultraviolet; Redshift; Extreme ultraviolet lithography; Context (archaeology); Sky","score_opus":0.01027053123924284,"score_gpt":0.21216802207279023,"score_spread":0.20189749083354738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2479368785","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99954057,0.00003875533,0.00008673818,0.0000053948083,6.5743336e-7,4.7963545e-7,0.00007752112,0.000004057008,0.00024575248],"genre_scores_gemma":[0.9998105,0.000012920768,0.000028993043,0.0000021698336,0.0000028698403,4.685735e-7,0.000104706705,7.715972e-7,0.00003656786],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988306,0.000021471567,0.0000072863863,0.000030474528,0.000025667365,0.000032036507],"domain_scores_gemma":[0.99873585,0.0003043874,0.0006388879,0.00008826236,0.000087533816,0.00014512379],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031136567,0.00010573141,0.00013428512,0.0009571379,0.00015428671,0.0004653306,0.00013757158,0.00014726148,0.0007369758],"category_scores_gemma":[0.0011504978,0.000067148954,0.00012489632,0.00065949676,0.00021193264,0.0002605926,0.00028900156,0.00016177486,0.00013128143],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056738547,0.000026091655,0.9899732,0.000006589389,0.000041140658,0.000087314496,0.00014757027,0.00028638606,0.0052868947,0.0001574627,0.00008552041,0.0038451261],"study_design_scores_gemma":[4.713041e-7,0.000012746521,0.9995253,8.914257e-7,0.0000024822755,0.000050438623,0.000027327058,0.00016657013,0.0001259262,0.000029668023,0.000057225076,9.4611556e-7],"about_ca_topic_score_codex":0.0012403511,"about_ca_topic_score_gemma":0.0012546446,"teacher_disagreement_score":0.0012403511,"about_ca_system_score_codex":0.00012366007,"about_ca_system_score_gemma":0.000037542923,"threshold_uncertainty_score":0.002466321},"labels":[],"label_agreement":null},{"id":"W2481623412","doi":"10.3847/0004-637x/826/1/92","title":"ROTATION AND GRANULATION OF THE K2 GIANT α SER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Granulation; Radial velocity; Line (geometry); Giant star; RADIUS; Spectrograph; Stars; Astronomy; Spectral line; Geometry","score_opus":0.007994004434180711,"score_gpt":0.2081504029799561,"score_spread":0.20015639854577538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2481623412","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965954,0.000012946099,0.000020479183,0.0000033246174,5.2737096e-7,9.536978e-7,0.00006410597,0.0000036403214,0.00023449434],"genre_scores_gemma":[0.99965596,0.000008668167,0.000029941119,0.0000048343854,0.0000013750432,0.0000010488798,0.00014287706,0.0000030056112,0.00015227441],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994326,0.0000054789402,0.0000038824987,0.000018843533,0.000009700551,0.000018787818],"domain_scores_gemma":[0.99963677,0.000032031152,0.00015329476,0.000041738265,0.00005422944,0.000081981685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014008886,0.00018934497,0.00015527273,0.0008070398,0.0003234109,0.0005319876,0.00012974323,0.00017222275,0.000800042],"category_scores_gemma":[0.000380907,0.0001368012,0.00014028548,0.0003755551,0.00035535614,0.00019860112,0.00035417188,0.00013359314,0.00032863533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004624007,0.000030043984,0.926675,0.000016687663,0.00003311331,0.00048943877,0.0006700869,0.0002473979,0.06693966,0.000053738215,0.0001724423,0.0042099836],"study_design_scores_gemma":[0.0000019223874,0.000021980593,0.9990495,9.567988e-7,0.0000026814973,0.00013355249,0.00006553575,0.000090499554,0.0004857728,0.0000098327855,0.00013604392,0.0000018077595],"about_ca_topic_score_codex":0.0045346827,"about_ca_topic_score_gemma":0.0058713336,"teacher_disagreement_score":0.0045346827,"about_ca_system_score_codex":0.00036255032,"about_ca_system_score_gemma":0.00008254894,"threshold_uncertainty_score":0.009016573},"labels":[],"label_agreement":null},{"id":"W2482920800","doi":"10.3847/0004-637x/826/2/138","title":"DOUBLE DYNAMO SIGNATURES IN A GLOBAL MHD SIMULATION AND MEAN-FIELD DYNAMOS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Dynamo; Physics; Solar dynamo; Differential rotation; Magnetohydrodynamics; Astrophysics; Dynamo theory; Convection zone; Magnetic field; Computational physics; Stars","score_opus":0.006668978894704451,"score_gpt":0.2539914872015072,"score_spread":0.24732250830680277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2482920800","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993905,0.000038963317,0.002494065,0.000154903,0.000015847172,0.00001916729,0.00032995743,0.00008618888,0.002955882],"genre_scores_gemma":[0.9984309,0.000020961363,0.0010193033,0.000025598134,0.0000053713948,0.000018849518,0.00022067907,0.000018417944,0.00023992555],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998971,0.000033343586,0.000005293794,0.000016827718,0.000018905195,0.000028523706],"domain_scores_gemma":[0.9994765,0.00027601977,0.00006055208,0.00004536162,0.00004924427,0.000092455135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031033077,0.000418211,0.00062554755,0.00041639266,0.0004327082,0.00087314844,0.0005854512,0.0009211953,0.0014203679],"category_scores_gemma":[0.0012521811,0.00023732416,0.00062600354,0.00032680912,0.00075079064,0.00036914015,0.00054948207,0.00068011606,0.00009727278],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014738442,0.0001273226,0.013054678,0.000021630094,0.000060521586,0.00018822154,0.00006848916,0.9816217,0.0016382497,0.0019163842,0.00028658978,0.0008688523],"study_design_scores_gemma":[0.000030973053,0.00003761927,0.0020611791,0.0000029965147,0.000007427678,0.000011006015,0.000027356778,0.9971468,0.000226499,0.00031237106,0.000130163,0.0000055893233],"about_ca_topic_score_codex":0.012147295,"about_ca_topic_score_gemma":0.0053257123,"teacher_disagreement_score":0.012147295,"about_ca_system_score_codex":0.0006622596,"about_ca_system_score_gemma":0.00059776194,"threshold_uncertainty_score":0.024153233},"labels":[],"label_agreement":null},{"id":"W2483741191","doi":"10.1088/0004-637x/809/1/80","title":"POPULATION SYNTHESIS OF CATACLYSMIC VARIABLES. I. INCLUSION OF DETAILED NUCLEAR EVOLUTION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Population; Astrophysics; Physics; Demography","score_opus":0.010368589304567634,"score_gpt":0.21937331679577088,"score_spread":0.20900472749120325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2483741191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.81170034,0.00069000036,0.17833525,0.0002441415,0.00013269263,0.00022547164,0.0025764592,0.00059373025,0.0055019553],"genre_scores_gemma":[0.9730794,0.00019993231,0.02218755,0.00007637392,0.000069119014,0.0002875392,0.0028662027,0.00014628853,0.0010876333],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99936265,0.0002337951,0.00003440574,0.00023009407,0.000082862614,0.000056159002],"domain_scores_gemma":[0.9980477,0.0009823189,0.00023058335,0.00040647105,0.00024673846,0.0000861392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001776389,0.0003882454,0.00069247605,0.00075049704,0.00055337325,0.0012310903,0.00078795536,0.00041314098,0.003488939],"category_scores_gemma":[0.006012332,0.00038215728,0.0011667623,0.0007013759,0.00036632878,0.0010072748,0.00094164157,0.00088939286,0.0003442762],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039852492,0.00011830943,0.17192088,0.0003275603,0.0011073833,0.0004204352,0.000816996,0.6735376,0.026203996,0.06121315,0.0019959456,0.06193922],"study_design_scores_gemma":[0.00008044555,0.00017734796,0.054341238,0.000020889236,0.00012696553,0.00014664014,0.00015820809,0.90862894,0.0055025807,0.021401616,0.009345591,0.00006951739],"about_ca_topic_score_codex":0.0030126066,"about_ca_topic_score_gemma":0.0018973995,"teacher_disagreement_score":0.003488939,"about_ca_system_score_codex":0.0009129264,"about_ca_system_score_gemma":0.00057778903,"threshold_uncertainty_score":0.011671603},"labels":[],"label_agreement":null},{"id":"W2485727682","doi":"10.3847/0004-637x/830/2/79","title":"A MECHANISM FOR STIMULATING AGN FEEDBACK BY LIFTING GAS IN MASSIVE GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Molecular cloud; Thermal; Stars; Millimeter; Star formation; Radiative cooling; Thermal equilibrium","score_opus":0.009520097977916945,"score_gpt":0.22686817983290944,"score_spread":0.2173480818549925,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2485727682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9761101,0.00050121424,0.012632723,0.0013000788,0.00013466115,0.000045933924,0.000103224076,0.0010828561,0.008089257],"genre_scores_gemma":[0.99806684,0.000045867146,0.00097322697,0.00008724158,0.000039961305,0.000013829844,0.000014626519,0.000009485599,0.00074886845],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999089,0.00001341503,0.0000048300694,0.00002036924,0.000019809648,0.00003264399],"domain_scores_gemma":[0.9995022,0.000089090194,0.00014256194,0.00006907111,0.000044393295,0.00015266873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027683302,0.00026794046,0.00021709355,0.00041376214,0.00039967956,0.0007814234,0.0007843154,0.00092996116,0.0042957477],"category_scores_gemma":[0.0009368633,0.00021632346,0.00029969978,0.000110478046,0.0004452076,0.0005815737,0.000661392,0.00031406048,0.00059036],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005391253,0.000366959,0.07775248,0.00038513198,0.00021408997,0.0033257639,0.0008155382,0.02444612,0.7979958,0.049875084,0.0058115856,0.038472306],"study_design_scores_gemma":[0.001120617,0.002274942,0.3162344,0.00017237524,0.00032325537,0.003683765,0.001314124,0.3940439,0.15472203,0.09424287,0.031661127,0.00020659852],"about_ca_topic_score_codex":0.0007595378,"about_ca_topic_score_gemma":0.0007126389,"teacher_disagreement_score":0.0042957477,"about_ca_system_score_codex":0.00055329734,"about_ca_system_score_gemma":0.0001957413,"threshold_uncertainty_score":0.01437068},"labels":[],"label_agreement":null},{"id":"W2485757243","doi":"10.3847/0004-637x/830/2/129","title":"SEARCH FOR SOURCES OF HIGH-ENERGY NEUTRONS WITH FOUR YEARS OF DATA FROM THE ICETOP DETECTOR","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; University of Oxford; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Pulsar; Astrophysics; Cosmic ray; Flux (metallurgy); Sky; Neutron star; Air shower; Neutron; Photon flux; Astronomy; Photon; Nuclear physics; Optics","score_opus":0.02380848942584076,"score_gpt":0.23619479436302165,"score_spread":0.2123863049371809,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2485757243","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99045146,0.00032358323,0.0027803308,0.000045436507,0.000011847227,0.00004151958,0.0036664912,0.000136439,0.0025428515],"genre_scores_gemma":[0.98087317,0.00011298686,0.0049410677,0.000053397638,0.000016032618,0.000038142356,0.012647016,0.000042922,0.0012751721],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99945694,0.0000802593,0.00004059484,0.00012503841,0.00014099707,0.00015615068],"domain_scores_gemma":[0.998145,0.00043631112,0.0005376067,0.00018355121,0.0003812244,0.00031639278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012099561,0.00038912412,0.0005995644,0.0020834792,0.0005180807,0.00076953124,0.00046638589,0.00053875404,0.0019141985],"category_scores_gemma":[0.001146486,0.0002959272,0.00055345526,0.0017861455,0.00013794318,0.0003783213,0.00072225794,0.00032195577,0.0005266693],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014564437,0.00038850665,0.92210525,0.00015086358,0.0006714797,0.0017604156,0.00017666628,0.0041843075,0.04196803,0.0003998225,0.0028922758,0.02384598],"study_design_scores_gemma":[0.00010720324,0.00052169815,0.93979234,0.000043548163,0.00038510922,0.0016792236,0.00027621078,0.014099223,0.032930437,0.00024956756,0.009870108,0.000045339577],"about_ca_topic_score_codex":0.0044237785,"about_ca_topic_score_gemma":0.0115578715,"teacher_disagreement_score":0.0044237785,"about_ca_system_score_codex":0.0004735315,"about_ca_system_score_gemma":0.00071109174,"threshold_uncertainty_score":0.008796036},"labels":[],"label_agreement":null},{"id":"W2486771893","doi":"10.3847/1538-4357/834/2/116","title":"PLANETARY ENGULFMENT AS A TRIGGER FOR WHITE DWARF POLLUTION","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":88,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Planetesimal; White dwarf; Physics; Planet; Astrophysics; Black dwarf; Accretion (finance); Astronomy; Planetary system; Metallicity; Astrobiology; Stars","score_opus":0.012331152741189106,"score_gpt":0.24368586513575488,"score_spread":0.2313547123945658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2486771893","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984465,0.00027605318,0.00042816935,0.00003211982,0.000007152508,0.0000052547753,0.00005746333,0.00004205181,0.00070524623],"genre_scores_gemma":[0.99961543,0.000039685117,0.000094621995,0.000010274211,0.0000038512862,0.0000017374774,0.00004812536,0.000002905629,0.00018337075],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998615,0.000013246256,0.000011765766,0.000039725484,0.000035710258,0.000038020586],"domain_scores_gemma":[0.99929917,0.00014012757,0.0002893813,0.000059603186,0.0000596942,0.00015210702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001984775,0.00018741748,0.0003351804,0.0005713772,0.00042424048,0.00061816024,0.00021134039,0.00045847674,0.0019632604],"category_scores_gemma":[0.0008186502,0.000112187445,0.00016161776,0.0002674734,0.00032555126,0.00042827008,0.00091071054,0.00035910102,0.0003275618],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007692025,0.00017476857,0.5772944,0.00018367487,0.00010415158,0.003638204,0.0005176622,0.0029231112,0.39401954,0.0020581454,0.00064493314,0.017672254],"study_design_scores_gemma":[0.000028753866,0.0005356238,0.91048896,0.000022461465,0.000054874294,0.004163559,0.00042932652,0.013453574,0.06573007,0.0016334482,0.0034391107,0.000020171286],"about_ca_topic_score_codex":0.0008341331,"about_ca_topic_score_gemma":0.0006964795,"teacher_disagreement_score":0.0019632604,"about_ca_system_score_codex":0.00040105262,"about_ca_system_score_gemma":0.00015315032,"threshold_uncertainty_score":0.006567776},"labels":[],"label_agreement":null},{"id":"W2486801944","doi":"10.3847/1538-4357/aa6c30","title":"Global Crustal Dynamics of Magnetars in Relation to Their Bright X-Ray Outbursts","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Magnetar; Crust; Physics; Geophysics; Neutron star; Creep; Magnetic field; Shear (geology); Astrophysics; Geology; Seismology; Mechanics; Petrology","score_opus":0.010652278059183451,"score_gpt":0.30861554839839167,"score_spread":0.2979632703392082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2486801944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99874544,0.0002666022,0.00009834674,0.00002076382,0.0000018700329,0.0000020787725,0.00012553047,0.0000112367525,0.00072821724],"genre_scores_gemma":[0.9994624,0.00010275759,0.000038335904,0.0000042981146,0.000004207821,0.000001263606,0.00017475372,0.0000047106346,0.00020730798],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.0000067199608,0.000004298868,0.000020080186,0.000009969416,0.000021924612],"domain_scores_gemma":[0.9995708,0.00004970818,0.00016778623,0.00003502013,0.000050348204,0.00012629153],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001904736,0.00030513067,0.00032473725,0.00077097834,0.00034468342,0.0008178817,0.00020588862,0.00025532805,0.0010661036],"category_scores_gemma":[0.00055457454,0.0001655435,0.00027255138,0.00041268577,0.0002653049,0.00032845963,0.0007459142,0.000296492,0.00022615778],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004570573,0.000032415486,0.95208484,0.000047014662,0.00014204526,0.0006242135,0.0007603407,0.0035398668,0.031488523,0.0003922261,0.00017927917,0.010252195],"study_design_scores_gemma":[0.0000024776225,0.00004963919,0.99809223,0.0000035961255,0.00001292272,0.00012519333,0.00017289468,0.0006641289,0.00045384222,0.00008833536,0.0003297851,0.0000049500704],"about_ca_topic_score_codex":0.0022569634,"about_ca_topic_score_gemma":0.0019498987,"teacher_disagreement_score":0.0022569634,"about_ca_system_score_codex":0.00030276002,"about_ca_system_score_gemma":0.00006723481,"threshold_uncertainty_score":0.0044876933},"labels":[],"label_agreement":null},{"id":"W2488323175","doi":"10.3847/0004-637x/831/2/133","title":"THE ERUPTION OF THE CANDIDATE YOUNG STAR ASASSN-15QI","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Photometry (optics); Stars; Spectral energy distribution; Accretion (finance); Emission spectrum; Flux (metallurgy); Spectral line; Be star","score_opus":0.0067627495723525536,"score_gpt":0.2247186223313243,"score_spread":0.21795587275897174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2488323175","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99830073,0.00008938447,0.00013733246,0.000017728964,0.0000077672385,0.000006144075,0.00012680443,0.000007115475,0.0013069927],"genre_scores_gemma":[0.99865365,0.000029362987,0.0002143469,0.00001637418,0.000005668207,0.0000020411596,0.00038504496,0.0000017200684,0.0006916504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999585,0.0000029293,0.0000024699546,0.000013157793,0.0000104301635,0.000012521533],"domain_scores_gemma":[0.99984,0.000014850864,0.000046761368,0.000010045733,0.000022074819,0.00006625608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012768342,0.00016273874,0.00016418764,0.00031220363,0.00041629243,0.00028710553,0.00010998453,0.00019817306,0.0012258546],"category_scores_gemma":[0.00014321221,0.00007427727,0.00017937039,0.00020622181,0.00018634247,0.00014599045,0.00023897651,0.00018401183,0.0002133769],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000104944585,0.00003383934,0.9412531,0.00004677509,0.00002464054,0.00097465445,0.0003526702,0.00016561114,0.048761144,0.00032309873,0.00036630133,0.007593165],"study_design_scores_gemma":[0.0000018627356,0.000058805963,0.9959009,0.000004495197,0.0000063815705,0.00037634955,0.00018250007,0.00025031474,0.0017746013,0.00004842365,0.0013931989,0.0000022129752],"about_ca_topic_score_codex":0.0020515928,"about_ca_topic_score_gemma":0.0054246276,"teacher_disagreement_score":0.0020515928,"about_ca_system_score_codex":0.00027452924,"about_ca_system_score_gemma":0.00012306661,"threshold_uncertainty_score":0.004100919},"labels":[],"label_agreement":null},{"id":"W2489883178","doi":"10.3847/0004-637x/830/2/103","title":"STELLAR ATMOSPHERES, ATMOSPHERIC EXTENSION, AND FUNDAMENTAL PARAMETERS: WEIGHING STARS USING THE STELLAR MASS INDEX","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Asteroseismology; Astrophysics; Angular diameter; Red supergiant; Stars; Stellar atmosphere; Supergiant; Stellar mass; Stellar evolution; Stellar mass loss; Stellar structure; Astronomy; RADIUS; Effective temperature; Giant star; Red giant; Binary star; Star formation","score_opus":0.01558394578318795,"score_gpt":0.22651281227423598,"score_spread":0.21092886649104803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2489883178","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9617774,0.00034502105,0.036082342,0.000035336616,0.0000074884524,0.000009160558,0.00020802123,0.00019917924,0.0013359922],"genre_scores_gemma":[0.99003977,0.000063746185,0.009632119,0.000006602029,0.000010382707,0.0000027311555,0.00014303498,0.000012733805,0.0000888626],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999728,0.00008248876,0.0000141127275,0.00008424061,0.00007675244,0.000014451149],"domain_scores_gemma":[0.99877495,0.00039922007,0.00039287968,0.00017661825,0.00013762587,0.00011870634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078670203,0.00035446946,0.0003088217,0.001855571,0.00021975781,0.0006874393,0.0003092392,0.00031791255,0.00027696686],"category_scores_gemma":[0.002515576,0.00019604428,0.00021589713,0.0009763542,0.00030287233,0.0009845477,0.0006612435,0.00026141305,0.00023354945],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000090804526,0.000045651544,0.9273487,0.000033342832,0.00015003695,0.000044229066,0.00009997771,0.010716994,0.02497011,0.00084936165,0.00020022437,0.03545069],"study_design_scores_gemma":[0.0000085350175,0.00008713193,0.8040271,0.000016083743,0.00005925516,0.00017505062,0.00008964677,0.17890322,0.01380246,0.0019594142,0.0008374462,0.000034746252],"about_ca_topic_score_codex":0.0013428847,"about_ca_topic_score_gemma":0.0023316727,"teacher_disagreement_score":0.001855571,"about_ca_system_score_codex":0.00022406786,"about_ca_system_score_gemma":0.00014885537,"threshold_uncertainty_score":0.0041605234},"labels":[],"label_agreement":null},{"id":"W2491593944","doi":"10.3847/0004-637x/829/2/73","title":"THE TWO CENTRAL STARS OF NGC 1514: CAN THEY ACTUALLY BE RELATED?*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Stars; Metallicity; Herbig Ae/Be star; Nebula; Binary star; Sky; Star (game theory); Radial velocity; Telescope; K-type main-sequence star","score_opus":0.008750112017116915,"score_gpt":0.21892367766479864,"score_spread":0.21017356564768172,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2491593944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9876659,0.0017169344,0.0007416046,0.0005295184,0.00019992802,0.000019098045,0.00008705519,0.000046132038,0.008993819],"genre_scores_gemma":[0.99719304,0.00021880752,0.00076884625,0.00021644816,0.00008199587,0.000010053221,0.00024533854,0.000009444847,0.0012560086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995148,0.00009584868,0.000045621153,0.0001525727,0.00007400526,0.00011719091],"domain_scores_gemma":[0.998268,0.0001833852,0.0006764207,0.0002605321,0.00031703894,0.00029465338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008279257,0.0004297923,0.0005954953,0.0010829794,0.0013400371,0.0013134112,0.0007690401,0.0016195448,0.0072072423],"category_scores_gemma":[0.0039967024,0.0002440843,0.00037981122,0.0010729817,0.0023408227,0.00157851,0.0012602613,0.00065607455,0.0022307625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000776591,0.00014268562,0.9076911,0.00029691335,0.00014091263,0.007625788,0.0027723035,0.00037140018,0.029010102,0.0068020658,0.0020251044,0.042345073],"study_design_scores_gemma":[0.000053480937,0.00031282907,0.9594373,0.0001279012,0.0000966915,0.010673408,0.0019357417,0.0006566565,0.0032291592,0.007298954,0.016126629,0.000051216455],"about_ca_topic_score_codex":0.0063070804,"about_ca_topic_score_gemma":0.0040058084,"teacher_disagreement_score":0.0072072423,"about_ca_system_score_codex":0.0012657209,"about_ca_system_score_gemma":0.0005129967,"threshold_uncertainty_score":0.024110615},"labels":[],"label_agreement":null},{"id":"W2491807675","doi":"10.3847/0004-637x/832/1/81","title":"APOCENTER GLOW IN ECCENTRIC DEBRIS DISKS: IMPLICATIONS FOR FOMALHAUT AND ϵ ERIDANI","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Debris disk; Eccentricity (behavior); Flux (metallurgy); Orbital eccentricity; Debris; Surface brightness; Brightness; Planetary system","score_opus":0.01117920204905565,"score_gpt":0.2525636553850558,"score_spread":0.24138445333600017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2491807675","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872406,0.00060974597,0.002085217,0.0014176288,0.000036455614,0.000015640013,0.00009684261,0.00009286434,0.008404886],"genre_scores_gemma":[0.999255,0.00005932269,0.0002656418,0.00006069185,0.00001926271,0.0000015462789,0.000020721287,0.0000039004944,0.00031392177],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998611,0.000020366828,0.000006677379,0.000051595714,0.000024704057,0.000035512996],"domain_scores_gemma":[0.9987709,0.00031084463,0.0004357162,0.00019354714,0.00011374535,0.000175272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061549,0.00025220716,0.00031363856,0.0004968949,0.0005797059,0.0010351583,0.0007797078,0.00085163943,0.0025795763],"category_scores_gemma":[0.0019333344,0.00016396126,0.00023750616,0.00039437576,0.0017743845,0.0012571316,0.0007546638,0.00035941423,0.0002782646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015169795,0.00018140429,0.8623055,0.0002553872,0.00008778373,0.0045913765,0.002867781,0.008288354,0.04808723,0.033140708,0.004166132,0.034511425],"study_design_scores_gemma":[0.00008185448,0.00014287308,0.93072915,0.000046148743,0.000052804895,0.0024740768,0.0027391175,0.026934799,0.0066919248,0.02437353,0.0056789294,0.000054692297],"about_ca_topic_score_codex":0.0028924153,"about_ca_topic_score_gemma":0.0020421145,"teacher_disagreement_score":0.0028924153,"about_ca_system_score_codex":0.0008658659,"about_ca_system_score_gemma":0.000147769,"threshold_uncertainty_score":0.008629501},"labels":[],"label_agreement":null},{"id":"W2491925477","doi":"10.3847/0004-637x/829/2/86","title":"A MEGACAM SURVEY OF OUTER HALO SATELLITES. VI. THE SPATIALLY RESOLVED STAR-FORMATION HISTORY OF THE CARINA DWARF SPHEROIDAL GALAXY*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Physics; Globular cluster; Milky Way; Star formation; Dwarf spheroidal galaxy; Stellar population; Metallicity; Dwarf galaxy; Local Group; Galaxy; Halo; Stellar mass; Astronomy; Photometry (optics); Population; RADIUS; Star cluster; Stars; Lenticular galaxy","score_opus":0.01844411633932095,"score_gpt":0.21119054465469744,"score_spread":0.1927464283153765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2491925477","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99325234,0.0004101266,0.00020299788,0.00003594447,0.0000039151514,0.000009809536,0.0028773313,0.000050961946,0.0031565428],"genre_scores_gemma":[0.99387544,0.000140101,0.0010162113,0.000025453068,0.000009948249,0.0000082190745,0.0037585087,0.000011079736,0.0011551005],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999254,0.000008415216,0.0000028658703,0.000025102696,0.00001745447,0.000020831416],"domain_scores_gemma":[0.9997017,0.000020992004,0.00007596122,0.000047071346,0.00006783913,0.000086539236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014816743,0.00017619005,0.00011900531,0.0009708413,0.00022130008,0.00024799258,0.00021378623,0.00015497084,0.0012065892],"category_scores_gemma":[0.00025796928,0.000098260156,0.00014361987,0.0005972864,0.000100807585,0.00016705402,0.00039140225,0.0001033019,0.0005363267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011342924,0.000029684867,0.95407045,0.000067667905,0.000071853996,0.00017945854,0.0004949668,0.00040758133,0.01461378,0.0002378204,0.0018507954,0.027862525],"study_design_scores_gemma":[0.0000023696175,0.000016219547,0.9945103,0.0000069520315,0.00000960021,0.00006493359,0.00008389042,0.0004475157,0.00059372,0.000020336443,0.004241625,0.0000023952416],"about_ca_topic_score_codex":0.024977358,"about_ca_topic_score_gemma":0.057094138,"teacher_disagreement_score":0.024977358,"about_ca_system_score_codex":0.00032746815,"about_ca_system_score_gemma":0.00019541403,"threshold_uncertainty_score":0},"labels":[],"label_agreement":null},{"id":"W2493324186","doi":"10.3847/0004-637x/830/1/35","title":"CHEMICAL ABUNDANCES IN A SAMPLE OF RED GIANTS IN THE OPEN CLUSTER NGC 2420 FROM APOGEE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Open cluster; Red giant; Abundance (ecology); Red-giant branch; Stars; Red clump; Giant star; Star cluster; Cluster (spacecraft)","score_opus":0.018550682045266303,"score_gpt":0.2518989546087277,"score_spread":0.23334827256346138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2493324186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939287,0.00003587651,0.000037873277,0.000005690478,9.062688e-7,0.0000033623996,0.0002915417,0.000009542744,0.00022236594],"genre_scores_gemma":[0.99717355,0.00004698989,0.00016819865,0.000020582427,0.000005774277,0.000009057395,0.0021707816,0.000011742331,0.00039338056],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997832,0.00002175957,0.000014006026,0.000080921665,0.00005522906,0.000044835353],"domain_scores_gemma":[0.99950254,0.000050901115,0.00012840965,0.000053197495,0.0000876984,0.00017717607],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025298263,0.0003455204,0.00023196779,0.0025898977,0.0005085849,0.00043972806,0.00033397088,0.0002463552,0.0011127848],"category_scores_gemma":[0.00071422645,0.00013740757,0.00016335033,0.0011462474,0.00036200273,0.00022573314,0.0009281186,0.000088412286,0.00040648205],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018802402,0.00007393418,0.9849412,0.000015889806,0.000043766766,0.00023225906,0.00064137956,0.00020260274,0.007859647,0.000079013946,0.00055994536,0.005162302],"study_design_scores_gemma":[0.00000449341,0.000022349619,0.99867815,0.0000018808774,0.000007491942,0.0000876819,0.00017902006,0.0001613637,0.00027051204,0.000020080017,0.00056425063,0.0000026180824],"about_ca_topic_score_codex":0.015017004,"about_ca_topic_score_gemma":0.020551402,"teacher_disagreement_score":0.015017004,"about_ca_system_score_codex":0.0005236961,"about_ca_system_score_gemma":0.00011884191,"threshold_uncertainty_score":0.029859185},"labels":[],"label_agreement":null},{"id":"W2493465271","doi":"10.3847/0004-637x/831/1/78","title":"IROCKS: SPATIALLY RESOLVED KINEMATICS OF z ∼ 1 STAR-FORMING GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Galaxy; Redshift; Star formation; Stellar population; Population; Kinematics; Stellar mass","score_opus":0.00943911661810211,"score_gpt":0.21435119986963644,"score_spread":0.20491208325153432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2493465271","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981791,0.000025360214,0.00014978682,0.000005769239,6.5198867e-7,0.000005136555,0.0011515953,0.000018418023,0.0004642005],"genre_scores_gemma":[0.99778396,0.000020993059,0.00029938383,0.000004993045,0.0000021752796,0.0000048586076,0.0017009577,0.000003983043,0.00017877638],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998367,0.000016363809,0.000010237161,0.000051662497,0.000032264943,0.000052677533],"domain_scores_gemma":[0.9994375,0.000040572184,0.00026971943,0.000051382878,0.0000701907,0.00013058113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002774074,0.00021509948,0.00020325945,0.0015412435,0.00017726311,0.0004958152,0.0002857246,0.00011359538,0.001211674],"category_scores_gemma":[0.00061439344,0.00012383566,0.00019686903,0.0007839824,0.0001794797,0.00025771532,0.00057672965,0.00016956283,0.0002476809],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050146857,0.000013747815,0.9937359,0.0000063846874,0.000017604192,0.000017234579,0.00015367768,0.00018536465,0.0030309178,0.0000865686,0.0001271622,0.0025753858],"study_design_scores_gemma":[0.0000017428683,0.000012590608,0.99923074,0.0000017951311,0.000005528797,0.000017522205,0.00008949548,0.00021147195,0.00025235454,0.000011874301,0.00016357345,0.0000013557508],"about_ca_topic_score_codex":0.01844171,"about_ca_topic_score_gemma":0.023253743,"teacher_disagreement_score":0.01844171,"about_ca_system_score_codex":0.00028064463,"about_ca_system_score_gemma":0.00014544855,"threshold_uncertainty_score":0.036668718},"labels":[],"label_agreement":null},{"id":"W2494963994","doi":"10.3847/0004-637x/830/2/144","title":"A BROWN DWARF CENSUS FROM THE SIMP SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Southern Hemisphere; Observatory; Sky; Northern Hemisphere; Telescope; Proper motion; Stellar classification","score_opus":0.020220204946534686,"score_gpt":0.2321436013845178,"score_spread":0.21192339643798314,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2494963994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9797615,0.00009957675,0.00043487156,0.000042631826,0.0000034281436,0.000031963886,0.015607242,0.0000713931,0.0039474047],"genre_scores_gemma":[0.9679633,0.00015054457,0.0009770875,0.000055650577,0.000015302727,0.00004627078,0.0278274,0.000034258985,0.0029301585],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997626,0.0000423431,0.000017452276,0.000067514025,0.00007360819,0.00003652387],"domain_scores_gemma":[0.999464,0.00005264524,0.00010262339,0.00008178667,0.00014663185,0.00015240962],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037569334,0.00016134875,0.0001228332,0.002364911,0.0002592687,0.00023414497,0.00021944541,0.00008794024,0.0032762869],"category_scores_gemma":[0.0006552216,0.00007243454,0.000093741335,0.0012352808,0.0001140096,0.00022877917,0.0005147156,0.000096873075,0.0014789454],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011192637,0.00002640451,0.9738858,0.000026181344,0.000014829779,0.00030237102,0.00031695943,0.00009938195,0.0038142034,0.00020461902,0.004546721,0.016650647],"study_design_scores_gemma":[0.0000042134798,0.000026701164,0.9926783,0.0000036053104,0.000004530045,0.00022003874,0.00017047067,0.00022438055,0.00062194426,0.00003812031,0.0060057603,0.0000017821387],"about_ca_topic_score_codex":0.01289841,"about_ca_topic_score_gemma":0.018388793,"teacher_disagreement_score":0.01289841,"about_ca_system_score_codex":0.00023898289,"about_ca_system_score_gemma":0.0002818749,"threshold_uncertainty_score":0.025646687},"labels":[],"label_agreement":null},{"id":"W2495424346","doi":"10.3847/1538-4357/aaca9b","title":"Constraints on the Distance Moduli, Helium and Metal Abundances, and Ages of Globular Clusters from their RR Lyrae and Non-variable Horizontal-branch Stars. III. M55 and NGC 6362","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"RR Lyrae variable; Physics; Globular cluster; Astrophysics; Horizontal branch; Stars; Moduli; Star cluster","score_opus":0.007048070835019206,"score_gpt":0.20041890740209126,"score_spread":0.19337083656707205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2495424346","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993081,0.00010289607,0.000058023008,0.000007104962,0.000001096436,9.4485966e-7,0.00007674647,0.000002348274,0.00044282235],"genre_scores_gemma":[0.99947697,0.000028932252,0.00009097702,0.000005457642,0.0000018884306,0.000001169384,0.00028508663,0.0000012324917,0.000108263026],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978346,0.000021680593,0.000022667868,0.00007205119,0.000050207862,0.00005002815],"domain_scores_gemma":[0.9992299,0.00019455551,0.00018948708,0.0000757294,0.00011282755,0.00019753621],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004882416,0.00038435822,0.00027353698,0.0011398417,0.0005032852,0.0006290612,0.00026795093,0.00037451417,0.0011981108],"category_scores_gemma":[0.0016424771,0.00020239635,0.0002256346,0.00043198426,0.00032143993,0.00030811972,0.0005854593,0.00013326845,0.0006064195],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017550075,0.00002145355,0.9822467,0.000018503095,0.000038370246,0.00008289475,0.00026300596,0.0005164636,0.011684557,0.000244683,0.00016167008,0.004546169],"study_design_scores_gemma":[0.0000064570436,0.00003861559,0.99775225,0.000007671081,0.000015459727,0.000053462685,0.00016891547,0.00077516306,0.0007469544,0.000090071844,0.00034126584,0.0000037993914],"about_ca_topic_score_codex":0.009676886,"about_ca_topic_score_gemma":0.017366394,"teacher_disagreement_score":0.009676886,"about_ca_system_score_codex":0.00048005508,"about_ca_system_score_gemma":0.00016919074,"threshold_uncertainty_score":0.019241095},"labels":[],"label_agreement":null},{"id":"W2495985119","doi":"10.3847/0004-637x/830/1/10","title":"OPTICAL IDENTIFICATION OF CEPHEIDS IN 19 HOST GALAXIES OF TYPE Ia SUPERNOVAE AND NGC 4258 WITH THE HUBBLE SPACE TELESCOPE*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Aspen Center for Physics; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Space Telescope Science Institute; Alfred P. Sloan Foundation; National Science Foundation","keywords":"Cepheid variable; Supernova; Galaxy; Hubble space telescope; Variable star; Homogeneous; Stars; Hubble sequence; Hubble's law","score_opus":0.008007092129838373,"score_gpt":0.22752919760244011,"score_spread":0.21952210547260173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2495985119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997192,0.000016361806,0.000054809654,0.0000011477968,3.3464426e-7,0.0000021704698,0.000047641395,0.000002801608,0.00015536402],"genre_scores_gemma":[0.9994879,0.000015287509,0.00018915173,0.0000025848378,0.000002058204,0.000002306922,0.00018485621,0.000001314328,0.000114592476],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997942,0.00003305531,0.000018965005,0.00006623744,0.000043467167,0.000044137785],"domain_scores_gemma":[0.99950695,0.00009753554,0.00014179516,0.00006190296,0.00005781734,0.0001340274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034835326,0.00020935883,0.00021902338,0.0016046927,0.00035998417,0.0004612553,0.00016329023,0.000135744,0.0008549177],"category_scores_gemma":[0.0005503262,0.00014214734,0.00014678162,0.00061101525,0.0002801399,0.0001918022,0.00047013597,0.00010082479,0.00015453716],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013387935,0.00003777292,0.9808004,0.000008110405,0.00003175573,0.00016490323,0.0002841693,0.000104269115,0.0141602075,0.000037134996,0.000041883763,0.004195671],"study_design_scores_gemma":[0.0000027003591,0.000045001998,0.9984779,7.8912444e-7,0.00001084488,0.00015048408,0.00013341423,0.00016957114,0.0008699759,0.000007993737,0.00012990614,0.0000015112564],"about_ca_topic_score_codex":0.0056708786,"about_ca_topic_score_gemma":0.013940875,"teacher_disagreement_score":0.0056708786,"about_ca_system_score_codex":0.00020373055,"about_ca_system_score_gemma":0.00014622562,"threshold_uncertainty_score":0.011275709},"labels":[],"label_agreement":null},{"id":"W2496510243","doi":"10.3847/0004-637x/826/2/222","title":"DIFFERENCES IN WATER VAPOR RADIATIVE TRANSFER AMONG 1D MODELS CAN SIGNIFICANTLY AFFECT THE INNER EDGE OF THE HABITABLE ZONE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Victoria","funders":"","keywords":"Physics; Solar constant; Radiative transfer; Circumstellar habitable zone; Atmospheric radiative transfer codes; Water vapor; Shortwave; Line (geometry); Atmospheric sciences; Longwave; Atmospheric model; Astrophysics; Exoplanet; Stars; Solar irradiance; Meteorology; Optics; Geometry","score_opus":0.011475481924973743,"score_gpt":0.21128075154502285,"score_spread":0.1998052696200491,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2496510243","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99400395,0.000059870654,0.004203692,0.00007718368,0.000011696861,0.000011508997,0.00032477046,0.00020975937,0.0010974507],"genre_scores_gemma":[0.99862874,0.00001514328,0.00094733865,0.000020966236,0.00000293955,0.000008062256,0.00022513114,0.00004262916,0.00010901549],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99962664,0.00013613743,0.000022558133,0.00010802459,0.000040740513,0.00006587886],"domain_scores_gemma":[0.9980556,0.0012385396,0.00017100715,0.00023685204,0.00016973689,0.00012833362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012412232,0.000696839,0.00058375316,0.0004239567,0.00039057893,0.0010888858,0.0011152327,0.000970692,0.0011474655],"category_scores_gemma":[0.0036880753,0.00032656867,0.0011052139,0.00032202914,0.0006176723,0.00091083767,0.000648482,0.00063603057,0.00020004704],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013988609,0.000059583894,0.04000313,0.000022338785,0.000126088,0.000049881015,0.000049966002,0.9540014,0.0026583655,0.00045104953,0.00022251575,0.0022157766],"study_design_scores_gemma":[0.000036301593,0.00003980207,0.01395199,0.000006394798,0.000035034976,0.000017051916,0.0000501928,0.98391473,0.0013447497,0.0003857002,0.00019569082,0.000022310507],"about_ca_topic_score_codex":0.027163625,"about_ca_topic_score_gemma":0.010964752,"teacher_disagreement_score":0.027163625,"about_ca_system_score_codex":0.0007264844,"about_ca_system_score_gemma":0.0005898617,"threshold_uncertainty_score":0.054011047},"labels":[],"label_agreement":null},{"id":"W2496839923","doi":"10.3847/0004-637x/829/1/5","title":"MAGNETIC FIELD DISORDER AND FARADAY EFFECTS ON THE POLARIZATION OF EXTRAGALACTIC RADIO SOURCES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Polarization (electrochemistry); Depolarization; Astrophysics; Redshift; Faraday cage; Faraday effect; Spectral index; Magnetic field; Sky; Spectral line; Astronomy; Galaxy","score_opus":0.003754729401736541,"score_gpt":0.18699398910226195,"score_spread":0.1832392597005254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2496839923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985317,0.000074689044,0.00022853234,0.000011832387,9.393915e-7,0.0000016284674,0.00053332216,0.000008100692,0.00060926215],"genre_scores_gemma":[0.9988319,0.000046460176,0.00007804664,0.000005251658,0.000004426238,0.0000016403216,0.0009377765,0.0000029367877,0.00009152134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996911,0.00009280081,0.000025126654,0.000057734538,0.00008413193,0.00004902961],"domain_scores_gemma":[0.99652594,0.0009459142,0.0014614749,0.00046706444,0.00039592944,0.00020373997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042482588,0.0001709114,0.00018852923,0.0016259707,0.0002352632,0.00059757737,0.00014250235,0.00014182471,0.0013047117],"category_scores_gemma":[0.0026579166,0.00010939962,0.00014651117,0.0013305956,0.0002462643,0.00032303896,0.0003988479,0.00011874606,0.00031200662],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059648533,0.000007462216,0.9935761,0.0000075705398,0.000020452742,0.000032216227,0.000033917193,0.00034358242,0.0026121316,0.0000747021,0.00008578125,0.0031465308],"study_design_scores_gemma":[0.0000016432293,0.0000057438633,0.99900925,0.0000017213885,0.0000049396244,0.000053636533,0.000019387482,0.0003248891,0.00040067706,0.00004554071,0.00013089577,0.0000015687461],"about_ca_topic_score_codex":0.0015759133,"about_ca_topic_score_gemma":0.0026621076,"teacher_disagreement_score":0.0016259707,"about_ca_system_score_codex":0.00019025289,"about_ca_system_score_gemma":0.00008555086,"threshold_uncertainty_score":0.004364729},"labels":[],"label_agreement":null},{"id":"W2496932746","doi":"10.3847/0004-637x/833/1/3","title":"OBSERVATION AND CHARACTERIZATION OF A COSMIC MUON NEUTRINO FLUX FROM THE NORTHERN HEMISPHERE USING SIX YEARS OF ICECUBE DATA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":510,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"Marsden Fund; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; University of Oxford; National Science Foundation; Compute Canada; Western Canada Research Grid; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Bundesministerium für Bildung und Forschung; Vetenskapsrådet; Villum Fonden","keywords":"Physics; Neutrino; Muon; Muon neutrino; Zenith; Flux (metallurgy); Cosmic ray; Neutrino detector; Neutrino astronomy; Astrophysics; Particle physics; Nuclear physics; Neutrino oscillation","score_opus":0.02328024496186829,"score_gpt":0.227249767645128,"score_spread":0.2039695226832597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2496932746","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98316664,0.00022727248,0.0010983658,0.000041381583,0.000011486813,0.000024643588,0.012741747,0.00011286484,0.0025757023],"genre_scores_gemma":[0.95815074,0.00023426014,0.002399872,0.00002852096,0.00002396375,0.00005231185,0.038643032,0.000065501525,0.00040176898],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965584,0.00006237212,0.000019400215,0.00009329126,0.00009426994,0.00007476023],"domain_scores_gemma":[0.99895346,0.00023157,0.00029029403,0.00017412752,0.00022429769,0.00012617865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010736044,0.00035846056,0.0004024173,0.0014264067,0.0003882219,0.0007944116,0.00031491288,0.0003096127,0.00083766686],"category_scores_gemma":[0.0010849424,0.00015285765,0.00047125277,0.0017079487,0.00028031654,0.00029818012,0.00046267634,0.0002448222,0.00026808179],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012739238,0.0001505692,0.9336031,0.00015735037,0.00036241443,0.0008051888,0.00055793475,0.0074045374,0.032032277,0.00049930124,0.0027197471,0.020433666],"study_design_scores_gemma":[0.000017877755,0.000056641402,0.9831118,0.000021586993,0.000054951215,0.0002725841,0.00008544249,0.0035309403,0.0070018345,0.00011748365,0.0057117343,0.00001708105],"about_ca_topic_score_codex":0.0137700485,"about_ca_topic_score_gemma":0.017621096,"teacher_disagreement_score":0.0137700485,"about_ca_system_score_codex":0.0005940628,"about_ca_system_score_gemma":0.000396118,"threshold_uncertainty_score":0.02737981},"labels":[],"label_agreement":null},{"id":"W2505541561","doi":"10.1088/0004-637x/811/2/133","title":"RAVEN AND THE CENTER OF MAFFEI 1: MULTI-OBJECT ADAPTIVE OPTICS OBSERVATIONS OF THE CENTER OF A NEARBY ELLIPTICAL GALAXY AND THE DETECTION OF AN INTERMEDIATE AGE POPULATION","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Galaxy; Stellar population; Subaru Telescope; Stars; Astronomy; Population; Spectral line; Spectrograph; Star formation","score_opus":0.026056989177988182,"score_gpt":0.23636133459572706,"score_spread":0.21030434541773887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2505541561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99201196,0.00043914944,0.0012592749,0.00006417137,0.000010582487,0.000010455049,0.00012248705,0.00008524642,0.00599682],"genre_scores_gemma":[0.99672264,0.00006620457,0.0018164134,0.00001735132,0.000009889314,0.0000043500722,0.00021948469,0.000008539509,0.0011351084],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998549,0.000015288499,0.0000035092528,0.00005918838,0.000039395563,0.000027624135],"domain_scores_gemma":[0.9997129,0.00003961914,0.00010852254,0.00003770824,0.000040865365,0.00006029887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034249175,0.00023895783,0.00015960528,0.00095025863,0.00047819928,0.00042725453,0.00034934317,0.00033706927,0.001188143],"category_scores_gemma":[0.00069096446,0.00018631155,0.0002332637,0.00023337337,0.0002761966,0.0005672495,0.0004759015,0.00029807808,0.00029042654],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048368634,0.000105890445,0.7610279,0.00008534802,0.00012614486,0.0008122461,0.0011640493,0.0013679889,0.17654352,0.0026695002,0.0020836864,0.05352998],"study_design_scores_gemma":[0.0000055689047,0.0000850968,0.9886874,0.000011871076,0.000013382161,0.00053548,0.000070366434,0.0013402497,0.006155416,0.00023459217,0.0028478943,0.000012717576],"about_ca_topic_score_codex":0.005138626,"about_ca_topic_score_gemma":0.013149792,"teacher_disagreement_score":0.005138626,"about_ca_system_score_codex":0.00043998804,"about_ca_system_score_gemma":0.00010087528,"threshold_uncertainty_score":0.010217428},"labels":[],"label_agreement":null},{"id":"W2505789590","doi":"10.3847/0004-637x/826/1/81","title":"INVESTIGATING THE CIRCUMSTELLAR DISK OF THE Be SHELL STAR 48 LIBRAE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Radiative transfer; Perturbation (astronomy); Oscillation (cell signaling); Observable; Be star; Star (game theory); Spectroscopy; Accretion disc","score_opus":0.013510958234525906,"score_gpt":0.22175997507534448,"score_spread":0.20824901684081856,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2505789590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972077,0.000054841836,0.0017939946,0.00002831728,0.0000038603443,0.000008736617,0.000093150156,0.00006978574,0.00073961396],"genre_scores_gemma":[0.99864906,0.000023629089,0.0009976494,0.000007134636,0.0000022243214,0.000004891294,0.00011727491,0.000023157747,0.0001750373],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999546,0.00000753761,0.0000035475505,0.000015885347,0.0000089345795,0.00000945475],"domain_scores_gemma":[0.9998796,0.000024270712,0.000019885763,0.000030089297,0.000015931824,0.000030156461],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010462786,0.0003493077,0.00029646602,0.00023856969,0.0003189937,0.00047621937,0.0005140746,0.0004035181,0.00069351855],"category_scores_gemma":[0.00044545784,0.00018535525,0.0004181614,0.00024327531,0.00024248286,0.00039201224,0.00048142686,0.00022337974,0.0002127656],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005445456,0.0003346749,0.2646385,0.00016299191,0.0002219225,0.002141187,0.0005293342,0.5351616,0.1776378,0.0034550813,0.000504325,0.014668063],"study_design_scores_gemma":[0.00011566884,0.00027140568,0.11175927,0.000009806895,0.000049976417,0.00031762387,0.00019681487,0.8672307,0.017870553,0.00067125005,0.0014740494,0.000032940097],"about_ca_topic_score_codex":0.0035459325,"about_ca_topic_score_gemma":0.0014212297,"teacher_disagreement_score":0.0035459325,"about_ca_system_score_codex":0.000489466,"about_ca_system_score_gemma":0.00016188534,"threshold_uncertainty_score":0.007050574},"labels":[],"label_agreement":null},{"id":"W2507954234","doi":"10.3847/0004-637x/830/2/58","title":"DETERMINATION OF CORONAL MASS EJECTION PHYSICAL PARAMETERS FROM A COMBINATION OF POLARIZED VISIBLE LIGHT AND UV Lyα OBSERVATIONS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Coronagraph; Coronal mass ejection; Extreme ultraviolet; Orbiter; Astrophysics; Observatory; Plasma; Spectral line; Extreme ultraviolet lithography; Solar radius; Astronomy; Solar wind; Optics; Exoplanet; Stars","score_opus":0.011250697222901288,"score_gpt":0.2286954901396129,"score_spread":0.21744479291671162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2507954234","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973116,0.000111813264,0.0011156854,0.0000068849927,0.0000023874773,0.000009547222,0.0003680472,0.000030026016,0.0010441387],"genre_scores_gemma":[0.9983954,0.0000577276,0.00094634894,0.0000052477053,0.0000052312216,0.000006872036,0.00048095256,0.000005337624,0.00009688264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993706,0.000007692595,0.0000029666337,0.000019104778,0.000019232375,0.000013947767],"domain_scores_gemma":[0.9998349,0.000035750367,0.0000490491,0.000011746226,0.000041374842,0.000027132292],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017046106,0.000248619,0.00016068167,0.0012455205,0.00016584907,0.0004312081,0.0001412052,0.00022480208,0.00037656768],"category_scores_gemma":[0.0002315782,0.000111247115,0.00018866142,0.0005650693,0.00011658847,0.00022541333,0.00017470935,0.00015207609,0.0001286765],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042718544,0.00008002562,0.6662166,0.000050913088,0.00009315539,0.0002455411,0.00009611695,0.0015185839,0.31405854,0.000077266326,0.0002084381,0.016927619],"study_design_scores_gemma":[0.000007398679,0.00004118219,0.9795497,0.000004712804,0.00002837275,0.00014327014,0.00007168014,0.00407365,0.015830453,0.000030471523,0.00021408431,0.0000050537437],"about_ca_topic_score_codex":0.0011693565,"about_ca_topic_score_gemma":0.0013468253,"teacher_disagreement_score":0.0012455205,"about_ca_system_score_codex":0.000119532444,"about_ca_system_score_gemma":0.000075351396,"threshold_uncertainty_score":0.0023251772},"labels":[],"label_agreement":null},{"id":"W2508009715","doi":"10.3847/1538-4357/833/1/93","title":"RETURN OF THE KING: TIME-SERIES PHOTOMETRY OF FO AQUARII’S INITIAL RECOVERY FROM ITS UNPRECEDENTED 2016 LOW STATE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Photometry (optics); Astrophysics; Brightness; Physics; Amplitude; Accretion disc; Polar; Intermediate polar; Cataclysmic variable star; Spectral line; Light curve; White dwarf; Astronomy; Stars; Optics","score_opus":0.010779922131325224,"score_gpt":0.2282015993066854,"score_spread":0.21742167717536018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508009715","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965659,0.000038618957,0.00038363965,0.00011917824,0.000012517454,0.0000066766756,0.00035375255,0.000050052535,0.0024696765],"genre_scores_gemma":[0.9989624,0.000010505754,0.00024374963,0.00002097184,0.00000799536,0.000002511412,0.00033910354,0.000007620282,0.00040518978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999182,0.000006672846,0.0000036859215,0.000020298918,0.00002779263,0.000023360259],"domain_scores_gemma":[0.99973446,0.000028811628,0.000058544618,0.000036135396,0.00006343623,0.0000786419],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026630922,0.00011680457,0.00019331009,0.00059257075,0.00046498142,0.00049847673,0.00022373591,0.0002930156,0.0012950117],"category_scores_gemma":[0.00055428705,0.00011649178,0.00012067633,0.00030055846,0.0002724976,0.00026261414,0.00039868124,0.00054021005,0.00037394816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087158085,0.00021127015,0.8000396,0.0000656635,0.00012791276,0.0015335903,0.0020490512,0.0015209231,0.15084329,0.0012938064,0.004449142,0.03699421],"study_design_scores_gemma":[0.00000507855,0.00005495384,0.99491113,0.0000038617,0.0000075193802,0.00016501339,0.00011309267,0.001280834,0.0018121414,0.000091579386,0.0015482096,0.000006601241],"about_ca_topic_score_codex":0.005461284,"about_ca_topic_score_gemma":0.009587091,"teacher_disagreement_score":0.005461284,"about_ca_system_score_codex":0.00044914393,"about_ca_system_score_gemma":0.00013418055,"threshold_uncertainty_score":0.010858953},"labels":[],"label_agreement":null},{"id":"W2508056928","doi":"10.3847/0004-637x/831/1/1","title":"CHEMODYNAMIC EVOLUTION OF DWARF GALAXIES IN TIDAL FIELDS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; Compute Canada","keywords":"Metallicity; Dwarf galaxy; Galaxy; Smoothed-particle hydrodynamics; Tidal force; Star formation; Gravitation; Gravitational potential","score_opus":0.0048697445293865915,"score_gpt":0.2005724393651259,"score_spread":0.1957026948357393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508056928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993266,0.000012184473,0.00024482503,0.00001901592,0.0000014993427,0.000002922991,0.00003614057,0.000018110837,0.000338835],"genre_scores_gemma":[0.9996111,0.000008487742,0.00016453346,0.0000070834067,7.596339e-7,0.0000020031252,0.000063241576,0.00000504924,0.00013792918],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999373,0.000014420332,0.000003967237,0.000014579993,0.000009052613,0.000020671898],"domain_scores_gemma":[0.9995091,0.00012244254,0.00008440059,0.0000520026,0.000075284814,0.0001567588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031816025,0.00020932531,0.00029790364,0.00053527264,0.00048661453,0.0008861303,0.0004199082,0.0003667414,0.0007233311],"category_scores_gemma":[0.0010692776,0.0002061599,0.0003764988,0.00035403785,0.0005774937,0.00033691715,0.0005359637,0.00027147873,0.00011289982],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003052084,0.00028258434,0.5189348,0.00003498833,0.00020302257,0.00041609682,0.0006527004,0.4456096,0.023494847,0.0039749118,0.0006684215,0.00542287],"study_design_scores_gemma":[0.000112783724,0.00018763517,0.22967248,0.000013545351,0.00006448292,0.00008630958,0.0003765435,0.76387423,0.0028152203,0.0019503037,0.000810824,0.0000356293],"about_ca_topic_score_codex":0.017735327,"about_ca_topic_score_gemma":0.009732247,"teacher_disagreement_score":0.017735327,"about_ca_system_score_codex":0.0011376549,"about_ca_system_score_gemma":0.00038986615,"threshold_uncertainty_score":0.035264194},"labels":[],"label_agreement":null},{"id":"W2508507187","doi":"10.3847/0004-637x/831/2/129","title":"FIRST DETECTION OF A PULSAR BOW SHOCK NEBULA IN FAR-UV: PSR J0437–4715<sup>∗</sup>","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Health Sciences Centre; Sunnybrook Health Science Centre","funders":"","keywords":"Pulsar; Bow shock (aerodynamics); Millisecond pulsar; Luminosity; Pulsar wind nebula; Nebula; Interstellar medium; Pulsar planet; Binary pulsar","score_opus":0.009838281552669489,"score_gpt":0.2791297170534976,"score_spread":0.2692914355008281,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508507187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949458,0.00051820284,0.0005914705,0.00007862062,0.00003413485,0.000011638988,0.00046606464,0.000083559244,0.0032704424],"genre_scores_gemma":[0.9978824,0.00007557234,0.00058205874,0.00006570894,0.000027276783,0.0000069215444,0.0006995998,0.0000148801955,0.00064553897],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999918,0.0000052273012,0.0000049481746,0.000021260463,0.000025031317,0.000025468387],"domain_scores_gemma":[0.9997714,0.000030773615,0.000054645396,0.000030318539,0.0000381601,0.00007465437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014970943,0.00021607218,0.00026251326,0.0005756376,0.0004721048,0.00061626104,0.0003599696,0.00043524744,0.003136304],"category_scores_gemma":[0.00024870533,0.0001667313,0.0002153979,0.00033217933,0.0002982913,0.00018021539,0.00042193837,0.00030120736,0.000658672],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007386302,0.00013888303,0.39766377,0.0002925231,0.00034945432,0.0076531316,0.00088582136,0.0004681557,0.549926,0.0011864989,0.0034918617,0.037205268],"study_design_scores_gemma":[0.000017418988,0.0003252913,0.96836287,0.000023289693,0.000072992894,0.0025667867,0.00024648802,0.00047522227,0.02017297,0.00023334881,0.0074908845,0.000012450129],"about_ca_topic_score_codex":0.0015623255,"about_ca_topic_score_gemma":0.0028496168,"teacher_disagreement_score":0.003136304,"about_ca_system_score_codex":0.0003648411,"about_ca_system_score_gemma":0.00014045225,"threshold_uncertainty_score":0.010491967},"labels":[],"label_agreement":null},{"id":"W2508548923","doi":"10.3847/0004-637x/819/2/170","title":"ERRATUM: “SPACING OF KEPLER PLANETS: SCUPLTING BY DYNAMICAL INSTABILITY” (2015, APJ, 807, 44)","year":2016,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Mathematics and Applications","field":"Mathematics","cited_by":5,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Kepler; Planet; Astronomy; Astrobiology; Instability; Astrophysics; Planetary system; Mechanics","score_opus":0.02071242757402223,"score_gpt":0.28924720711212876,"score_spread":0.2685347795381065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508548923","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00035434304,0.0008147321,0.0005113215,0.03540855,0.95306146,0.000015905514,0.0014772068,0.00037224678,0.007984151],"genre_scores_gemma":[0.024292927,0.007029497,0.005679012,0.072512664,0.38178205,0.00014584872,0.007950255,0.0026178008,0.49798995],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99742436,0.00023268699,0.0005608144,0.0004910175,0.0011075085,0.0001836282],"domain_scores_gemma":[0.98966473,0.0019343735,0.0008151009,0.0010585813,0.0058906907,0.0006365028],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020390053,0.002759943,0.0017940437,0.0039471313,0.0047683856,0.004356583,0.0035072363,0.0049789636,0.060146194],"category_scores_gemma":[0.033112533,0.0011755135,0.0016363208,0.0025012018,0.0024850776,0.004391663,0.0025058112,0.0066970373,0.046005778],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045746703,0.000008692097,0.00013319217,0.00006198331,0.000008555763,0.00014395821,0.00002417598,0.00006644741,0.00008991646,0.0016427246,0.99364775,0.0041267895],"study_design_scores_gemma":[0.000042905176,0.00004618686,0.0025116403,0.0002610679,0.000041119973,0.0004391404,0.00016566624,0.00048118795,0.0006859116,0.0056847963,0.9895773,0.00006306045],"about_ca_topic_score_codex":0.020477295,"about_ca_topic_score_gemma":0.020864647,"teacher_disagreement_score":0.060146194,"about_ca_system_score_codex":0.004132412,"about_ca_system_score_gemma":0.003895326,"threshold_uncertainty_score":0.20120907},"labels":[],"label_agreement":null},{"id":"W2508792583","doi":"10.3847/1538-4357/aa6db4","title":"Testing for X-Ray–SZ Differences and Redshift Evolution in the X-Ray Morphology of Galaxy Clusters","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Fermilab; High Energy Physics; Smithsonian Astrophysical Observatory; Office of Science; Ames Research Center; Strong; University of Chicago; Argonne National Laboratory; U.S. Department of Energy; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Universities Space Research Association; Smithsonian Institution; Yale University; National Science Foundation","keywords":"Astrophysics; ROSAT; Redshift; Physics; Galaxy cluster; Galaxy; South Pole Telescope; Morphology (biology); Cluster (spacecraft); X-ray; Asymmetry; Telescope; Optics; Biology","score_opus":0.01780099283201899,"score_gpt":0.24092403393045994,"score_spread":0.22312304109844094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508792583","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943095,0.000012363699,0.0003176242,0.000007681006,6.288098e-7,0.0000024877595,0.00010179557,0.0000084589665,0.0001180444],"genre_scores_gemma":[0.99961495,0.0000034366983,0.00016802551,0.0000020813027,0.0000010144241,0.0000021784153,0.00016632964,0.000003338003,0.00003851334],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99892163,0.00034792445,0.00007256068,0.0002831588,0.00026792372,0.000106844316],"domain_scores_gemma":[0.9912369,0.0049199485,0.0018395376,0.0008911743,0.00044209787,0.0006703331],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015990996,0.00027326666,0.00021404504,0.0009850458,0.000280734,0.0008531766,0.00054576463,0.0003746058,0.0015631976],"category_scores_gemma":[0.007719973,0.00019628182,0.00043539456,0.0007118579,0.0007150733,0.00058683165,0.0006753429,0.00032862904,0.00019563347],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000663978,0.00008234712,0.96844125,0.00001803029,0.00025628548,0.000063984655,0.00009845674,0.006645802,0.020671157,0.00026028784,0.00007807943,0.0027204074],"study_design_scores_gemma":[0.0000115451685,0.00012260917,0.98609215,0.0000013430302,0.000023170796,0.000058995727,0.00008112818,0.0100899525,0.0033500807,0.00006439857,0.00009931192,0.0000053464996],"about_ca_topic_score_codex":0.0018606635,"about_ca_topic_score_gemma":0.0013128457,"teacher_disagreement_score":0.0018606635,"about_ca_system_score_codex":0.00041892927,"about_ca_system_score_gemma":0.00017418189,"threshold_uncertainty_score":0.008456945},"labels":[],"label_agreement":null},{"id":"W2508825552","doi":"10.3847/0004-637x/831/1/49","title":"FROM EXOPLANETS TO QUASARS: DETECTION OF POTENTIAL DAMPED Lyα ABSORBING GALAXIES USING ANGULAR DIFFERENTIAL IMAGING","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Galaxy; Photometry (optics); Redshift; Quasar; Telescope; Photometric redshift; Exoplanet; Angular diameter","score_opus":0.0071897166383839365,"score_gpt":0.2109762230749352,"score_spread":0.20378650643655125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508825552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99548316,0.000108598964,0.0027893407,0.000020518966,0.0000016532113,0.000008332588,0.00014546665,0.00007739045,0.0013655655],"genre_scores_gemma":[0.9987326,0.000024331352,0.0010537023,0.000011148823,0.0000018769392,0.0000027155531,0.0000787948,0.0000031953916,0.000091509624],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999033,0.000014014629,0.00000545958,0.000033849825,0.000020717931,0.000022610862],"domain_scores_gemma":[0.99960417,0.000113652364,0.000110855945,0.000042419484,0.000038252263,0.000090743524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000312999,0.00019348972,0.00013400358,0.000843518,0.0001619559,0.0006345145,0.00023174961,0.00014516922,0.0011584691],"category_scores_gemma":[0.0005192732,0.0001568842,0.00015687343,0.00042243864,0.00021949311,0.00025945617,0.00046932467,0.000217442,0.00018358877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020515507,0.000047896472,0.8430018,0.000050894683,0.000052147996,0.00028912898,0.00019329136,0.00081367453,0.136826,0.00027129505,0.00011988601,0.018128935],"study_design_scores_gemma":[0.000005216344,0.0001047499,0.981006,0.000006054956,0.000023752978,0.0005324247,0.00016503032,0.004428606,0.013103258,0.00019444674,0.00042200607,0.000008401425],"about_ca_topic_score_codex":0.000888769,"about_ca_topic_score_gemma":0.0017849868,"teacher_disagreement_score":0.0011584691,"about_ca_system_score_codex":0.00018386293,"about_ca_system_score_gemma":0.000047594465,"threshold_uncertainty_score":0.003875494},"labels":[],"label_agreement":null},{"id":"W2508987369","doi":"10.3847/0004-637x/832/1/12","title":"ANALYSIS OF THE HERSCHEL/HEXOS SPECTRAL SURVEY TOWARD ORION SOUTH: A MASSIVE PROTOSTELLAR ENVELOPE WITH STRONG EXTERNAL IRRADIATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics; University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada; Stockholms Universitet; Chalmers Tekniska Högskola; Eidgenössische Technische Hochschule Zürich; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Deutsche Forschungsgemeinschaft","keywords":"Physics; Astrophysics; Ridge; Trace gas; Molecular cloud; Envelope (radar); Submillimeter Array; Spectral line; Observatory; Star formation; Astronomy; Atmospheric sciences; Stars","score_opus":0.01733139908363468,"score_gpt":0.23550455003453244,"score_spread":0.21817315095089776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2508987369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992483,0.000023646857,0.00010912413,0.000008984421,7.282681e-7,0.0000019868876,0.000287475,0.0000121103185,0.00030769617],"genre_scores_gemma":[0.9985037,0.00002644096,0.00033610733,0.000013364301,0.0000053559284,0.0000034597563,0.0009602601,0.000011500878,0.00013988135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998696,0.000017562143,0.000004822193,0.000046278066,0.000040280887,0.000021531994],"domain_scores_gemma":[0.99951005,0.00008061522,0.00017589235,0.0000644471,0.000059643968,0.00010934357],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026523357,0.00026656632,0.0002080564,0.000835335,0.00026239562,0.00033128052,0.00021697703,0.00017415466,0.00065857155],"category_scores_gemma":[0.00034366135,0.0001320241,0.00023296675,0.0005400311,0.00023255352,0.00015862125,0.00039626946,0.00014196298,0.00021066381],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015585685,0.000035963356,0.94873184,0.00002430712,0.000076445605,0.00026501523,0.00025983315,0.00065046403,0.04373922,0.000095386655,0.00023900703,0.005726849],"study_design_scores_gemma":[0.000005622591,0.000015866573,0.99731475,0.0000025106676,0.000014059474,0.00008634142,0.00006559275,0.00068768713,0.0013399221,0.000016346397,0.00044862938,0.0000025293264],"about_ca_topic_score_codex":0.0055830507,"about_ca_topic_score_gemma":0.009239536,"teacher_disagreement_score":0.0055830507,"about_ca_system_score_codex":0.00026086927,"about_ca_system_score_gemma":0.0001536661,"threshold_uncertainty_score":0.011101127},"labels":[],"label_agreement":null},{"id":"W2509488157","doi":"10.3847/1538-4357/aa5da6","title":"The Interaction of Relativistic Spacecrafts with the Interstellar Medium","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Spacecraft; Physics; Interstellar medium; Comet; Cosmic dust; Evaporation; Astrophysics; Astrobiology; Atomic physics; Astronomy; Meteorology","score_opus":0.011767777222956424,"score_gpt":0.2541002701213761,"score_spread":0.24233249289841968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2509488157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929617,0.0002809992,0.0034762416,0.000037846905,0.000015590556,0.000014586717,0.000050144165,0.00007007523,0.0030927444],"genre_scores_gemma":[0.9991762,0.000047694597,0.00039672144,0.0000086701975,0.0000028675493,0.0000026471323,0.00002602897,0.000007077894,0.00033210238],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998197,0.00002607812,0.0000053095223,0.000029319353,0.000060015347,0.000059491373],"domain_scores_gemma":[0.999587,0.0001474096,0.00010655778,0.00005074072,0.00005087795,0.00005740122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029101555,0.0004293466,0.00031064515,0.00061203673,0.00057569495,0.00070341787,0.00047839235,0.0005025745,0.0015350452],"category_scores_gemma":[0.00075202907,0.00023814198,0.0003822152,0.0003312101,0.000589206,0.00049964077,0.0008533058,0.00040973673,0.00014779913],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051335397,0.00024871615,0.09146047,0.00019186844,0.00038164473,0.0022154853,0.00038694264,0.58501905,0.3027775,0.005266311,0.0005991199,0.010939599],"study_design_scores_gemma":[0.00009764665,0.0015355529,0.18874733,0.000036413323,0.00021326952,0.0010887268,0.00078429986,0.7118276,0.09017279,0.0022535408,0.0031270967,0.000115781564],"about_ca_topic_score_codex":0.0031413573,"about_ca_topic_score_gemma":0.0022190963,"teacher_disagreement_score":0.0031413573,"about_ca_system_score_codex":0.0008993937,"about_ca_system_score_gemma":0.00017741749,"threshold_uncertainty_score":0.006525576},"labels":[],"label_agreement":null},{"id":"W2509534862","doi":"10.3847/1538-4357/833/2/264","title":"THE BOSS EMISSION-LINE LENS SURVEY. IV. SMOOTH LENS MODELS FOR THE BELLS GALLERY SAMPLE*","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Japan Society for the Promotion of Science; Chinese Academy of Sciences; U.S. Department of Energy; National Natural Science Foundation of China; York University; Space Telescope Science Institute; Carnegie Mellon University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Ministry of Education, Culture, Sports, Science and Technology; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; National Aeronautics and Space Administration; Brookhaven National Laboratory","keywords":"Physics; Astrophysics; Redshift; Galaxy; Lens (geology); Einstein radius; RADIUS; Astronomy; Line (geometry); Quasar; Gravitational lens; Optics","score_opus":0.028245153931919818,"score_gpt":0.2452937478568035,"score_spread":0.21704859392488368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2509534862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98969203,0.0003564979,0.00081288733,0.000112198446,0.000003286694,0.00001788272,0.00746096,0.000050370556,0.0014938543],"genre_scores_gemma":[0.98939437,0.000091216825,0.0005545604,0.000018803812,0.0000072529865,0.000008851984,0.009145894,0.00001680228,0.00076229085],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995516,0.00010166349,0.000028692384,0.00011141277,0.0000724352,0.00013416637],"domain_scores_gemma":[0.9989427,0.00010291594,0.0005091394,0.00014194992,0.00009465215,0.0002087269],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013905262,0.0004930924,0.00033833517,0.0016803489,0.00038387487,0.0007299387,0.0005807229,0.0002311789,0.0038528114],"category_scores_gemma":[0.001140446,0.0002436063,0.00056131417,0.0012069627,0.00023962058,0.0005525321,0.00088686054,0.00016525347,0.0010657111],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017000515,0.000013179512,0.9908043,0.000013178721,0.000113514485,0.000053500717,0.00008456446,0.0006498704,0.00059094396,0.00057791086,0.0014420584,0.0054868837],"study_design_scores_gemma":[0.00001464299,0.000042280924,0.99132055,0.00000740192,0.000048911224,0.00005545461,0.00017293634,0.0059341122,0.00017928098,0.00023049986,0.0019866882,0.0000072739786],"about_ca_topic_score_codex":0.05410692,"about_ca_topic_score_gemma":0.08265689,"teacher_disagreement_score":0.05410692,"about_ca_system_score_codex":0.0007978829,"about_ca_system_score_gemma":0.0003124564,"threshold_uncertainty_score":0.10758394},"labels":[],"label_agreement":null},{"id":"W2509584094","doi":"10.3847/1538-4357/833/2/186","title":"THE THERMAL STATE OF KS 1731−260 AFTER 14.5 YEARS IN QUIESCENCE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Neutron star; Thermal; Cooling curve; Thermal conductivity; Crust; Thermal state; Stars; Thermal equilibrium","score_opus":0.0068179593252147,"score_gpt":0.21295482767782653,"score_spread":0.20613686835261183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2509584094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989221,0.000042401698,0.00009209215,0.000011122072,0.0000024400933,0.0000027483939,0.00034129,0.000028616943,0.0005572777],"genre_scores_gemma":[0.9992092,0.00001158068,0.000081421575,0.0000071580394,0.0000017030947,0.0000016220633,0.0004930536,0.000007562567,0.00018678527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999318,0.0000035739088,0.0000027348904,0.000020955908,0.000013211318,0.000027733486],"domain_scores_gemma":[0.9997625,0.000024567868,0.000077317985,0.00002020892,0.000046577006,0.00006878235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017257914,0.00029026737,0.00034783673,0.0005922938,0.00046996438,0.0004631697,0.00027938586,0.0003144086,0.0013791755],"category_scores_gemma":[0.0002844241,0.0001575854,0.00031673693,0.0004522555,0.00025402484,0.00020418035,0.00025591295,0.00034017922,0.00031993297],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012305169,0.00013200108,0.8418916,0.00006616506,0.00013889658,0.0010610572,0.0005453909,0.003849864,0.13859276,0.0003940588,0.0007268998,0.011370836],"study_design_scores_gemma":[0.0000055312607,0.00005807089,0.9942253,0.000004008994,0.000014911222,0.00013371516,0.00009534236,0.0010297239,0.003896057,0.00003498236,0.0004924098,0.000009882634],"about_ca_topic_score_codex":0.014601667,"about_ca_topic_score_gemma":0.018888619,"teacher_disagreement_score":0.014601667,"about_ca_system_score_codex":0.00093785016,"about_ca_system_score_gemma":0.00022804177,"threshold_uncertainty_score":0.029033363},"labels":[],"label_agreement":null},{"id":"W2509720109","doi":"10.3847/0004-637x/832/2/109","title":"BOW TIES IN THE SKY. I. THE ANGULAR STRUCTURE OF INVERSE COMPTON GAMMA-RAY HALOS IN THE FERMI SKY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Industry Canada; National Science Foundation; Government of Canada; Klaus Tschira Stiftung; National Aeronautics and Space Administration","keywords":"Physics; Cosmic microwave background; Fermi Gamma-ray Space Telescope; Compton scattering; Gamma ray; Halo; Astrophysics; Photon; Sky; Population; Electron; Anisotropy; Astronomy; Nuclear physics; Galaxy; Optics","score_opus":0.007810965156951817,"score_gpt":0.2130473302832474,"score_spread":0.2052363651262956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2509720109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9558455,0.00043084702,0.018980494,0.00016839306,0.000012647124,0.000016132659,0.00021195051,0.0001708683,0.024163216],"genre_scores_gemma":[0.99761295,0.000050414663,0.0014637837,0.000012179645,0.0000065036575,0.0000024171152,0.000069361835,0.000012932021,0.00076947815],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999325,0.00001302063,0.0000030470906,0.000016521597,0.000013053963,0.000021686928],"domain_scores_gemma":[0.99966395,0.00006611798,0.00010033294,0.000047340713,0.000045708442,0.00007649601],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021611564,0.00015389279,0.00010677082,0.0009671712,0.00028565517,0.0009652868,0.00017797679,0.00015101688,0.002849159],"category_scores_gemma":[0.0010425658,0.00015201462,0.00016919362,0.0005115906,0.00060910697,0.00047124492,0.0006331279,0.00023998412,0.00021126524],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074340065,0.00008431505,0.33335385,0.00016674156,0.00013996728,0.0017538703,0.0021552288,0.05676132,0.09561677,0.40640074,0.004849815,0.097973965],"study_design_scores_gemma":[0.000075453456,0.00015742626,0.7199683,0.000086209264,0.0000781223,0.0019752092,0.0011442715,0.10685785,0.017556358,0.13873576,0.013297634,0.000067419656],"about_ca_topic_score_codex":0.0023853749,"about_ca_topic_score_gemma":0.0018343463,"teacher_disagreement_score":0.002849159,"about_ca_system_score_codex":0.00039161672,"about_ca_system_score_gemma":0.00014653437,"threshold_uncertainty_score":0.009531379},"labels":[],"label_agreement":null},{"id":"W2510024875","doi":"10.3847/0004-637x/829/1/33","title":"A SURVEY OF LUMINOUS HIGH-REDSHIFT QUASARS WITH SDSS AND WISE. II. THE BRIGHT END OF THE QUASAR LUMINOSITY FUNCTION AT z ∼ 5","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; University of Portsmouth; University of California, Los Angeles; Chinese Academy of Sciences; U.S. Department of Energy; National Natural Science Foundation of China; York University; Carnegie Mellon University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; People's Government of Yunnan Province; New Mexico State University; Yale University; Vanderbilt University; National Science Foundation; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory","keywords":"Quasar; Astrophysics; Redshift; Physics; Luminosity function; Sky; Luminosity; OVV quasar; Astronomy; Cosmology; Galaxy","score_opus":0.007851185201061182,"score_gpt":0.1894621221912054,"score_spread":0.18161093699014422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510024875","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967681,0.00019871817,0.00064738904,0.00002517051,0.0000034237455,0.000010816496,0.0015014685,0.000039520597,0.00080536265],"genre_scores_gemma":[0.9936504,0.00010429058,0.0012553879,0.000036327965,0.000009096424,0.000008310722,0.00456695,0.000007630676,0.00036160377],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973184,0.000039042297,0.000024350307,0.00006484732,0.00008223058,0.000057678822],"domain_scores_gemma":[0.9991849,0.000063051935,0.0003028338,0.0000726715,0.00012156314,0.00025497194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061437266,0.00024793964,0.00019018217,0.0018917279,0.00025335944,0.00046812007,0.0002341452,0.00014223966,0.0008934094],"category_scores_gemma":[0.00054789195,0.0001712094,0.0002736225,0.0010402323,0.000194318,0.00036136262,0.00054640276,0.00018416629,0.00033068637],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030486031,0.00002840012,0.98875415,0.000015385755,0.00004957946,0.00004710668,0.00012850875,0.00012535,0.003435907,0.00016450082,0.000408054,0.0068125683],"study_design_scores_gemma":[0.000001626556,0.000012860672,0.99897504,0.0000019013356,0.000006729374,0.00003564673,0.00004380393,0.00015379493,0.00018946546,0.000013453339,0.0005643969,0.0000013563014],"about_ca_topic_score_codex":0.007642553,"about_ca_topic_score_gemma":0.016272461,"teacher_disagreement_score":0.007642553,"about_ca_system_score_codex":0.00024409151,"about_ca_system_score_gemma":0.00017991458,"threshold_uncertainty_score":0.015196145},"labels":[],"label_agreement":null},{"id":"W2510077309","doi":"10.3847/0004-637x/828/2/113","title":"ALMA OBSERVATIONS OF THE DEBRIS DISK OF SOLAR ANALOG τ CETI","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Debris disk; Photosphere; Flux (metallurgy); Angular diameter; Debris; Planet; Millimeter; Planetesimal","score_opus":0.017710173783826052,"score_gpt":0.2314921553116239,"score_spread":0.21378198152779784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510077309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940999,0.00010042613,0.0003526373,0.000038753813,0.000008154901,0.000006426729,0.0005432727,0.00007437869,0.004775997],"genre_scores_gemma":[0.99860865,0.000025673304,0.00056018005,0.000016870494,0.000010997737,0.0000031880982,0.00042669772,0.000005902737,0.00034190324],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994683,0.000003818858,0.0000022277454,0.000017860373,0.000016583714,0.000012635718],"domain_scores_gemma":[0.9997873,0.000027794822,0.00006048294,0.000031500047,0.00003753409,0.000055460674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001437943,0.00011594366,0.00012965061,0.0004856324,0.000367523,0.00030055473,0.0002016111,0.00017474883,0.0014196363],"category_scores_gemma":[0.00035480366,0.000112965405,0.00015265272,0.00025570687,0.00010369806,0.00017529621,0.00026575098,0.00026123214,0.00031238433],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079193694,0.0001637387,0.75493664,0.00008821894,0.00013894944,0.0005479692,0.00069536036,0.0013071804,0.19696328,0.0013764526,0.0026032992,0.040386986],"study_design_scores_gemma":[0.00002079932,0.00008249584,0.98958594,0.0000073765905,0.000026101705,0.00018191515,0.00008620725,0.002097301,0.004663541,0.00013877582,0.003103927,0.000005502317],"about_ca_topic_score_codex":0.0018910384,"about_ca_topic_score_gemma":0.0031060893,"teacher_disagreement_score":0.0018910384,"about_ca_system_score_codex":0.00031745312,"about_ca_system_score_gemma":0.000082973376,"threshold_uncertainty_score":0.0047491193},"labels":[],"label_agreement":null},{"id":"W2510171012","doi":"10.3847/1538-4357/834/1/72","title":"TWO LONG-TERM INTERMITTENT PULSARS DISCOVERED IN THE PALFA SURVEY","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Office of Naval Research; National Aeronautics and Space Administration; Canada Research Chairs; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Science Foundation","keywords":"Pulsar; Population; Millisecond pulsar; Intermittency; Duty cycle; Neutron star; Polar cap; Observatory","score_opus":0.0333486657905208,"score_gpt":0.376075556900189,"score_spread":0.3427268911096682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510171012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99765414,0.00015909947,0.00038290807,0.00004851454,0.000010108074,0.0000059158524,0.00020069597,0.000029867488,0.0015087473],"genre_scores_gemma":[0.99852175,0.00007936362,0.00033481757,0.000035720648,0.000019523859,0.000006971638,0.00060103746,0.000005316646,0.0003955477],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986506,0.000012556714,0.00000668073,0.000036597732,0.000037570564,0.000041509717],"domain_scores_gemma":[0.9994019,0.00007868324,0.0002019001,0.000060999402,0.00009937156,0.00015709398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002618391,0.0001579445,0.00015386975,0.0010396319,0.0004248777,0.0005212965,0.00027246875,0.00024119025,0.0010176033],"category_scores_gemma":[0.00045879456,0.00010484248,0.00015208697,0.0005352303,0.00028020726,0.00025192453,0.0005463749,0.0003104527,0.00032205984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019209612,0.00007155552,0.94872385,0.00003843065,0.0000650573,0.0013018269,0.00055990316,0.00011820982,0.028731894,0.00024481385,0.00059514365,0.019357221],"study_design_scores_gemma":[0.000005799299,0.000056004737,0.9961357,0.0000045278925,0.000011891266,0.00045077785,0.00012355654,0.0001312212,0.0006346207,0.000032668522,0.0024093727,0.000003959367],"about_ca_topic_score_codex":0.0025039096,"about_ca_topic_score_gemma":0.0049606985,"teacher_disagreement_score":0.0025039096,"about_ca_system_score_codex":0.00026903555,"about_ca_system_score_gemma":0.00016204595,"threshold_uncertainty_score":0.0049787164},"labels":[],"label_agreement":null},{"id":"W2510282348","doi":"10.1088/0004-637x/815/2/135","title":"ERRATUM: “HERMES: ALMA IMAGING OF <i>HERSCHEL</i>-SELECTED DUSTY STAR-FORMING GALAXIES” (2015, ApJ, 812, 43)","year":2015,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Ancient Mediterranean Archaeology and History","field":"Arts and Humanities","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Galaxy; Astrophysics; Star (game theory); Astronomy","score_opus":0.021294881216138598,"score_gpt":0.22887479851124148,"score_spread":0.2075799172951029,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510282348","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.002678579,0.0014920627,0.0017039956,0.0469304,0.91401243,0.000057637342,0.009277761,0.0020310706,0.02181599],"genre_scores_gemma":[0.04470067,0.005576354,0.013058753,0.06769859,0.11942254,0.00017286894,0.041977655,0.007507204,0.6998853],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9981364,0.00012398596,0.00030095378,0.00028629377,0.0010222932,0.00012999466],"domain_scores_gemma":[0.9947464,0.00077668315,0.0005609855,0.00049339846,0.0029839328,0.00043858378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001478124,0.0016310168,0.0010983099,0.0041112746,0.0039320816,0.003141701,0.00194508,0.0034697703,0.05852293],"category_scores_gemma":[0.0122165065,0.0010616786,0.0011014637,0.0021694584,0.0014998771,0.0019394036,0.0019443829,0.004959138,0.028561212],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036710662,0.000014557482,0.00026017174,0.00004882062,0.00001038591,0.00019491167,0.000037001515,0.000054799908,0.00020816618,0.00044293547,0.9941303,0.004561243],"study_design_scores_gemma":[0.000036334528,0.000026049687,0.0046009994,0.0001922135,0.00004145293,0.0004001953,0.00013716954,0.00032401603,0.0011313406,0.0010832812,0.9919682,0.000058767397],"about_ca_topic_score_codex":0.029815348,"about_ca_topic_score_gemma":0.052295372,"teacher_disagreement_score":0.05852293,"about_ca_system_score_codex":0.003536187,"about_ca_system_score_gemma":0.0030826838,"threshold_uncertainty_score":0.19577867},"labels":[],"label_agreement":null},{"id":"W2510745844","doi":"10.3847/1538-4357/833/1/102","title":"FIRST SEASON MWA EOR POWER SPECTRUM RESULTS AT REDSHIFT 7","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":170,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; Pipeline (software); Redshift; Spectral density; Limit (mathematics); Large Synoptic Survey Telescope; Data set; Power (physics); Figure of merit","score_opus":0.006056902757822014,"score_gpt":0.2001656925899933,"score_spread":0.1941087898321713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510745844","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9038489,0.00055064185,0.030381652,0.000917194,0.00015686887,0.00006555234,0.030654322,0.0083926795,0.02503219],"genre_scores_gemma":[0.93925965,0.00010217836,0.018129244,0.00017503486,0.00009505577,0.00003324365,0.033581633,0.0014445818,0.0071794717],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99927133,0.00007521244,0.00003169461,0.0001774252,0.0003299893,0.00011437704],"domain_scores_gemma":[0.99611723,0.00049078313,0.00047389435,0.0011433065,0.0013163934,0.00045832744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012731397,0.0005519444,0.00046276723,0.0020185788,0.00033497787,0.0011184019,0.0003826257,0.00038238557,0.0043190205],"category_scores_gemma":[0.002320143,0.0002166184,0.0007117108,0.0008451057,0.00020605062,0.0006457963,0.0009339356,0.0006303056,0.0032097525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010894316,0.00038376782,0.6488828,0.00027603432,0.0007411127,0.0009585708,0.0010474983,0.0136022875,0.10892462,0.0074663935,0.06486315,0.15176432],"study_design_scores_gemma":[0.000044014483,0.00009583905,0.9239124,0.00003323389,0.00009722434,0.0003668596,0.00018914847,0.019361416,0.022493063,0.002023315,0.031319275,0.00006417574],"about_ca_topic_score_codex":0.0038737585,"about_ca_topic_score_gemma":0.006788829,"teacher_disagreement_score":0.0043190205,"about_ca_system_score_codex":0.00043351518,"about_ca_system_score_gemma":0.00014910412,"threshold_uncertainty_score":0.0144485235},"labels":[],"label_agreement":null},{"id":"W2510793222","doi":"10.3847/0004-637x/831/1/31","title":"A SUBTLE INFRARED EXCESS ASSOCIATED WITH A YOUNG WHITE DWARF IN THE EDINBURGH-CAPE BLUE OBJECT SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Montreal Clinical Research Institute","funders":"","keywords":"White dwarf; Infrared excess; Infrared; Opacity; Atmosphere (unit); Spectroscopy; Proper motion; Infrared spectroscopy; Cosmic infrared background","score_opus":0.01383301575281384,"score_gpt":0.23290241303697615,"score_spread":0.2190693972841623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510793222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992817,0.000044274308,0.000037756592,0.000018756095,0.000001918806,0.0000014867186,0.00016046558,0.0000032320972,0.0004504267],"genre_scores_gemma":[0.99956065,0.00003414873,0.00005752339,0.000010134143,0.0000033306228,9.802467e-7,0.00015298619,0.00000123847,0.0001789315],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984694,0.000012564153,0.00001135736,0.00004290603,0.00005139991,0.0000348405],"domain_scores_gemma":[0.99941075,0.00006289669,0.00027822287,0.00004784015,0.000054917098,0.00014538344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020408888,0.00015878679,0.0001626593,0.0010752887,0.0002803692,0.00039704557,0.00025771654,0.00015539478,0.0009969714],"category_scores_gemma":[0.0006715495,0.00010552996,0.000094018505,0.00067947304,0.00043275047,0.00022783403,0.0005268239,0.00011085626,0.00014581584],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007460706,0.000009745839,0.98508483,0.000017724906,0.00002312341,0.00077572,0.00042428996,0.000042129755,0.010540052,0.000084945925,0.0002609021,0.0026619297],"study_design_scores_gemma":[0.0000010026464,0.0000059271083,0.999398,0.0000014954753,0.0000033140561,0.00015247223,0.000097695556,0.000018144114,0.00013358671,0.000009046221,0.00017828924,9.949072e-7],"about_ca_topic_score_codex":0.021919627,"about_ca_topic_score_gemma":0.040413655,"teacher_disagreement_score":0.021919627,"about_ca_system_score_codex":0.0002935197,"about_ca_system_score_gemma":0.00014593909,"threshold_uncertainty_score":0.04358411},"labels":[],"label_agreement":null},{"id":"W2510875474","doi":"10.3847/0004-637x/830/2/139","title":"FORMATION AND EVOLUTION OF BLUE STRAGGLERS IN 47 TUCANAE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Blue straggler; Physics; Stars; Astrophysics; Stellar evolution; Asymptotic giant branch; Star cluster; Astronomy; Population","score_opus":0.007624400165134028,"score_gpt":0.2047145767677781,"score_spread":0.19709017660264408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2510875474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99916637,0.00008131922,0.0000385128,0.000008486718,0.0000016987134,0.0000021624203,0.00012962903,0.0000059456947,0.0005658824],"genre_scores_gemma":[0.9990626,0.000049069626,0.00009574813,0.000007471618,0.0000015936859,0.00000259687,0.00037377462,0.000004094835,0.000403088],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998394,0.000008353057,0.000005890453,0.000044284614,0.00003319299,0.00006899532],"domain_scores_gemma":[0.9997317,0.000020740901,0.0000615548,0.000017344355,0.00007989474,0.00008881804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018518054,0.00020908174,0.00030329882,0.003358027,0.0015678186,0.00088293274,0.00040658377,0.00042992528,0.0013065534],"category_scores_gemma":[0.00040685377,0.00015005202,0.00020946446,0.0019654478,0.00073700846,0.00023474784,0.0006094318,0.00024392376,0.00028673868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015273411,0.000047162954,0.9620198,0.000016601574,0.000042979475,0.0003768381,0.0008201307,0.00052087265,0.024323743,0.0002533883,0.00018649628,0.011239343],"study_design_scores_gemma":[0.0000016016322,0.000014487028,0.9974141,0.0000028833367,0.0000087041835,0.000098302975,0.00036052096,0.00038123547,0.00087398017,0.000040414627,0.0007989907,0.000004694632],"about_ca_topic_score_codex":0.19634618,"about_ca_topic_score_gemma":0.21412405,"teacher_disagreement_score":0.19634618,"about_ca_system_score_codex":0.0018796204,"about_ca_system_score_gemma":0.00085236155,"threshold_uncertainty_score":0.3904066},"labels":[],"label_agreement":null},{"id":"W2511877802","doi":"10.3847/0004-637x/833/1/12","title":"VLA AND ALMA IMAGING OF INTENSE GALAXY-WIDE STAR FORMATION IN z ∼ 2 GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Chulalongkorn University; National Science Council; National Institutes of Natural Sciences; FP7 Space; Japan Society for the Promotion of Science; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Ministry of Education, Culture, Sports, Science and Technology; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Luminous infrared galaxy; Lenticular galaxy; Peculiar galaxy","score_opus":0.0059182723963504364,"score_gpt":0.20301788827037992,"score_spread":0.1970996158740295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2511877802","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99791485,0.000090142035,0.0004912681,0.00001976358,0.0000022574409,0.0000037755085,0.00038993574,0.0000719572,0.0010158825],"genre_scores_gemma":[0.99860376,0.000016624039,0.00061450026,0.000016336911,0.000006582925,0.000003507948,0.00045584762,0.0000068393642,0.0002760806],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999101,0.000008740415,0.000003444296,0.000024492632,0.000021225149,0.00003193424],"domain_scores_gemma":[0.9997328,0.00003661621,0.00006378531,0.000024759516,0.00004435216,0.000097693985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002227126,0.00013094899,0.0001531991,0.0017069547,0.0001988613,0.00040211575,0.0001952926,0.00020360104,0.0013213942],"category_scores_gemma":[0.0002814246,0.00015271809,0.00018062688,0.00042514192,0.00011895119,0.00018341938,0.00030077086,0.00014213107,0.00026388714],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046182834,0.00008866926,0.7397215,0.000039670398,0.00011732717,0.0003494136,0.00027926738,0.00069360423,0.2421401,0.00031233198,0.00090625766,0.01489006],"study_design_scores_gemma":[0.000005688651,0.000030427835,0.9967062,0.0000026274056,0.000010262281,0.00013440353,0.000045026114,0.00094248593,0.0017240507,0.000040647374,0.0003553387,0.0000028483444],"about_ca_topic_score_codex":0.0023631991,"about_ca_topic_score_gemma":0.0057624234,"teacher_disagreement_score":0.0023631991,"about_ca_system_score_codex":0.00025663327,"about_ca_system_score_gemma":0.00007616382,"threshold_uncertainty_score":0.0046988726},"labels":[],"label_agreement":null},{"id":"W2512192954","doi":"10.3847/0004-637x/831/2/155","title":"A VLA SURVEY FOR FAINT COMPACT RADIO SOURCES IN THE ORION NEBULA CLUSTER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Physics; Millimeter; Astrophysics; Orion Nebula; Nebula; Cluster (spacecraft); Flux (metallurgy); Wavelength; Astronomy; Molecular cloud; Optics; Stars","score_opus":0.020888629029505366,"score_gpt":0.2632054931962941,"score_spread":0.24231686416678874,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2512192954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995127,0.00004984494,0.000079988604,0.000009156253,8.7037216e-7,0.000002921417,0.0001378027,0.000009070887,0.00019771878],"genre_scores_gemma":[0.99883014,0.00003692863,0.00033490625,0.0000052491946,0.0000052247524,0.0000041941644,0.0006051468,0.00000483513,0.0001733788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998641,0.000013641718,0.000007448289,0.000048744627,0.000041951345,0.000024097086],"domain_scores_gemma":[0.9993349,0.00007990447,0.00021444054,0.00006307752,0.00007923442,0.00022849598],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003064481,0.00022274593,0.00024035739,0.0019131893,0.00045132163,0.00045496968,0.00028373292,0.00016662067,0.000714967],"category_scores_gemma":[0.00057473686,0.00014116749,0.00013495596,0.0009019945,0.00021877521,0.00019023802,0.00054942997,0.00012899077,0.00014346752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008483197,0.000045213696,0.9836198,0.000011973036,0.000046484616,0.000125222,0.0003626603,0.00046448017,0.0077035814,0.00013928911,0.00029730712,0.007099058],"study_design_scores_gemma":[0.000002365171,0.000009552861,0.99907756,0.0000026085827,0.0000059336226,0.0000415821,0.0000619165,0.00036135662,0.00014870189,0.000021083515,0.00026525013,0.000002052088],"about_ca_topic_score_codex":0.0110034635,"about_ca_topic_score_gemma":0.023243614,"teacher_disagreement_score":0.0110034635,"about_ca_system_score_codex":0.00044675934,"about_ca_system_score_gemma":0.00022738782,"threshold_uncertainty_score":0.021878839},"labels":[],"label_agreement":null},{"id":"W2512827041","doi":"10.3847/1538-4357/aa7060","title":"Observed Faraday Effects in Damped Lyα Absorbers and Lyman Limit Systems: The Magnetized Environment of Galactic Building Blocks at Redshift = 2","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Office of Science; University of Toronto; Alfred P. Sloan Foundation; Associated Universities; University of Minnesota; U.S. Department of Energy; National Radio Astronomy Observatory; National Science Foundation","keywords":"Faraday effect; Redshift; Quasar; Polarization (electrochemistry); Magnetic field; Faraday cage; Dynamo; Galaxy; Sky","score_opus":0.013230451287178585,"score_gpt":0.21787184050144606,"score_spread":0.20464138921426747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2512827041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918884,0.000014877284,0.00028337532,0.000010250911,6.0018783e-7,0.0000016211364,0.000154046,0.000011389711,0.00033507383],"genre_scores_gemma":[0.99964786,0.000004112164,0.000101470345,0.0000053430363,0.0000020014995,0.0000013975357,0.0001743187,0.0000023807233,0.00006118695],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969804,0.000045048226,0.000016698343,0.00009763797,0.00006302526,0.0000795953],"domain_scores_gemma":[0.9980963,0.00038408994,0.000761609,0.0001963293,0.00017128719,0.00039041505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042087602,0.0002979397,0.0002622003,0.0011604998,0.0003242086,0.0007870739,0.00025454685,0.00030227317,0.0017372187],"category_scores_gemma":[0.0011975238,0.0001305433,0.00029615298,0.0005407538,0.0004222818,0.00028143078,0.00049726135,0.00020437513,0.00023465676],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009827744,0.000044572134,0.9791356,0.000009224817,0.000053749343,0.00004795131,0.000075571435,0.00048741797,0.018500384,0.00013971877,0.00007161458,0.0013358914],"study_design_scores_gemma":[0.0000041898993,0.000017816286,0.99778676,9.261086e-7,0.000010807165,0.000031269097,0.000045544148,0.0006644882,0.0012825059,0.00006675812,0.00008583823,0.000003062126],"about_ca_topic_score_codex":0.005155613,"about_ca_topic_score_gemma":0.0046665133,"teacher_disagreement_score":0.005155613,"about_ca_system_score_codex":0.00033704695,"about_ca_system_score_gemma":0.000094278315,"threshold_uncertainty_score":0.010251224},"labels":[],"label_agreement":null},{"id":"W2513124424","doi":"10.3847/1538-4357/833/2/229","title":"OBSERVATIONAL EVIDENCE OF DYNAMIC STAR FORMATION RATE IN MILKY WAY GIANT MOLECULAR CLOUDS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":152,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Milky Way; Star formation; Astrophysics; Molecular cloud; Virial mass; CMB cold spot; Stars; Velocity dispersion; Star (game theory); Sigma; Virial theorem; Astronomy; Galaxy; Cosmic microwave background","score_opus":0.022585878965072536,"score_gpt":0.26487765890502113,"score_spread":0.2422917799399486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2513124424","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99964774,0.00005011332,0.000056191147,0.000011116392,6.4408107e-7,7.6639344e-7,0.00011502186,0.000003241741,0.00011520761],"genre_scores_gemma":[0.9997198,0.000019152923,0.00003453074,0.0000026481734,0.00000202644,6.224823e-7,0.00020029268,0.0000013240128,0.000019646393],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996418,0.00006422256,0.000032909586,0.000105513835,0.00008473652,0.000070813105],"domain_scores_gemma":[0.9950158,0.0008725137,0.002531256,0.0006537222,0.00041639275,0.0005103505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068563444,0.0001170127,0.00031878846,0.0015584448,0.00030380904,0.0007845553,0.0004056691,0.00034909297,0.0005289546],"category_scores_gemma":[0.0036212709,0.00019641173,0.00025109103,0.001687431,0.00055253133,0.00070531183,0.0007408402,0.00023765296,0.00010982775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000026068792,0.000005562363,0.997726,0.0000051641346,0.000032407854,0.000020682914,0.00009469756,0.00014112615,0.0011447304,0.00008277498,0.000037803835,0.0006829659],"study_design_scores_gemma":[0.0000011987802,0.0000074723466,0.99943453,0.0000018136896,0.0000054183347,0.000034082055,0.00004582836,0.00023396045,0.00012670076,0.000029354242,0.00007786408,0.000001663161],"about_ca_topic_score_codex":0.009079557,"about_ca_topic_score_gemma":0.009364468,"teacher_disagreement_score":0.009079557,"about_ca_system_score_codex":0.00043983874,"about_ca_system_score_gemma":0.00017759351,"threshold_uncertainty_score":0.018053412},"labels":[],"label_agreement":null},{"id":"W2513167827","doi":"10.3847/1538-4357/833/2/192","title":"TIMING OF FIVE PALFA-DISCOVERED MILLISECOND PULSARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Office of Naval Research; National Aeronautics and Space Administration; Canada Research Chairs; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Science Foundation","keywords":"Millisecond pulsar; Pulsar; Neutron star; Binary pulsar; Astrometry; Binary number; Binary star","score_opus":0.014511236738867169,"score_gpt":0.30491247573456465,"score_spread":0.2904012389956975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2513167827","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973295,0.00015778649,0.00024334724,0.000028117418,0.000008098937,0.000010310788,0.0007025361,0.00002461595,0.0014957201],"genre_scores_gemma":[0.9967372,0.000094271476,0.0005720073,0.000018862314,0.000013312748,0.000013369467,0.0019910499,0.0000062600625,0.00055368914],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997855,0.000015671714,0.000014966411,0.000057059784,0.00007871059,0.000048064827],"domain_scores_gemma":[0.9989988,0.00012343495,0.00040359132,0.00006310083,0.00025365688,0.0001573373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002875323,0.0001784412,0.00018642689,0.001567885,0.00050299335,0.0004624583,0.00026566128,0.00020762242,0.0012987308],"category_scores_gemma":[0.00085048826,0.00012392827,0.00013413308,0.0007364152,0.00019252207,0.00019717561,0.0005193902,0.00025976283,0.00032190362],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023358596,0.000040250623,0.9674685,0.000043110438,0.000047132115,0.00038757845,0.0003712142,0.0001222612,0.013993435,0.00015430816,0.00051709515,0.016621348],"study_design_scores_gemma":[0.0000049277473,0.00006165147,0.99614245,0.0000044943667,0.000009430704,0.00026362602,0.0000842307,0.00012951727,0.0014721466,0.000021660739,0.0018024488,0.000003474753],"about_ca_topic_score_codex":0.004648652,"about_ca_topic_score_gemma":0.010372581,"teacher_disagreement_score":0.004648652,"about_ca_system_score_codex":0.000429703,"about_ca_system_score_gemma":0.00018286477,"threshold_uncertainty_score":0.00924319},"labels":[],"label_agreement":null},{"id":"W2513362382","doi":"10.3847/0004-637x/831/2/139","title":"A RADIAL AGE GRADIENT IN THE GEOMETRICALLY THICK DISK OF THE MILKY WAY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Science and Technology Facilities Council; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; European Commission; U.S. Department of Energy","keywords":"Milky Way; Physics; Astrophysics; Thick disk; Thin disk; Galaxy; Stars; Disc; Astronomy; Galaxy formation and evolution; Halo","score_opus":0.011792511632036389,"score_gpt":0.2164376784305939,"score_spread":0.2046451667985575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2513362382","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877733,0.00022217198,0.00015014397,0.000030376737,0.0000024103042,9.597435e-7,0.00011167014,0.00000903699,0.00069588906],"genre_scores_gemma":[0.9995123,0.0000521639,0.00010459963,0.000010629482,0.000002635592,7.382919e-7,0.00014518647,0.0000036219733,0.00016816937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999021,0.00001594413,0.0000070626456,0.000037595793,0.000017553704,0.000019715822],"domain_scores_gemma":[0.9991202,0.00011118788,0.00039179737,0.000076704906,0.00017382589,0.00012630096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002352679,0.00013304118,0.00014614672,0.0007790988,0.00022743031,0.0006107436,0.00018521215,0.00025298094,0.0011648673],"category_scores_gemma":[0.0012038477,0.000099369674,0.00013076443,0.0004179916,0.00033046448,0.00048489135,0.00056810945,0.00013355163,0.0003283754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007991361,0.000008889575,0.9853035,0.000014815048,0.000033833454,0.00012555078,0.00030926356,0.00041502545,0.008228447,0.00052569056,0.00019373346,0.0047613955],"study_design_scores_gemma":[0.000001449757,0.000012958428,0.9985582,0.0000038612907,0.0000062950553,0.00010104559,0.00013521986,0.00016783844,0.00032742549,0.00014378494,0.0005389401,0.0000029922492],"about_ca_topic_score_codex":0.0027608238,"about_ca_topic_score_gemma":0.0033382808,"teacher_disagreement_score":0.0027608238,"about_ca_system_score_codex":0.0002334713,"about_ca_system_score_gemma":0.000086984866,"threshold_uncertainty_score":0.005489528},"labels":[],"label_agreement":null},{"id":"W2514163811","doi":"10.3847/0004-637x/831/1/11","title":"THE AGE AND DISTANCE OF THE KEPLER OPEN CLUSTER NGC 6811 FROM AN ECLIPSING BINARY, TURNOFF STAR PULSATION, AND GIANT ASTEROSEISMOLOGY<sup>∗</sup>","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Jet Propulsion Laboratory; Office of Science; Ludwig-Maximilians-Universität München; Georg-August-Universität Göttingen; Universität Wien; National Aeronautics and Space Administration; Stellar Astrophysics Centre; Danmarks Grundforskningsfond; York University; Space Telescope Science Institute; Villum Fonden; Ohio State University; National Research Foundation; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Curtin University of Technology; U.S. Department of Energy; Aarhus Universitet; Harvard University; San Diego State University; New Mexico State University; University of Portsmouth; Science Mission Directorate; Yale University; Vanderbilt University; National Science Foundation","keywords":"Stars; Open cluster; Blue straggler; Star cluster; Hertzsprung–Russell diagram; Cluster (spacecraft); Binary star; Primary (astronomy)","score_opus":0.012406571579862767,"score_gpt":0.23616805789393103,"score_spread":0.22376148631406825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2514163811","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993637,0.000011141876,0.000033930464,0.000006254856,8.074397e-7,6.240886e-7,0.00018588362,0.0000023848406,0.00039529044],"genre_scores_gemma":[0.9990128,0.000009468294,0.000038439626,0.0000020422715,0.0000015577822,0.0000011444553,0.00071695173,0.0000024661813,0.00021505043],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999895,0.000010345506,0.0000060958905,0.000029518524,0.000025819147,0.00003321098],"domain_scores_gemma":[0.99927145,0.00016680374,0.00017501,0.00005584935,0.00013265542,0.00019815653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001439135,0.00019192512,0.00014702325,0.00089045876,0.00041265826,0.00044468613,0.00020286642,0.00022751122,0.0019589122],"category_scores_gemma":[0.00080137805,0.00008260257,0.00012031187,0.00045829694,0.00021184637,0.0002039105,0.00032745724,0.00018949884,0.00057486206],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000080256366,0.000013706121,0.9950428,0.000004245844,0.00001374016,0.0001461724,0.00009152636,0.00034302377,0.002384934,0.000053465013,0.00015507085,0.0016710162],"study_design_scores_gemma":[9.288757e-7,0.000011658732,0.9991097,6.966824e-7,0.000005105237,0.000094247735,0.000081708255,0.00025779134,0.0001916203,0.000014431555,0.00023021974,0.000001865381],"about_ca_topic_score_codex":0.0156126935,"about_ca_topic_score_gemma":0.021612132,"teacher_disagreement_score":0.0156126935,"about_ca_system_score_codex":0.00044055795,"about_ca_system_score_gemma":0.00018451642,"threshold_uncertainty_score":0.031043649},"labels":[],"label_agreement":null},{"id":"W2514242314","doi":"10.3847/0004-637x/830/2/99","title":"THE ACS FORNAX CLUSTER SURVEY. XII. DIFFUSE STAR CLUSTERS IN EARLY-TYPE GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Fornax Cluster; Surface brightness; Star cluster; Galaxy; Cluster (spacecraft); Virgo Cluster; Galaxy cluster; Elliptical galaxy","score_opus":0.010230755694924936,"score_gpt":0.21673614699370783,"score_spread":0.2065053912987829,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2514242314","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3921344,0.0060941502,0.0003952006,0.000866712,0.00017989748,0.00035565667,0.56503606,0.00089780596,0.03404014],"genre_scores_gemma":[0.4215005,0.0037665926,0.0018562631,0.00035903614,0.00039291184,0.00031979536,0.5558685,0.00016372427,0.015772609],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996693,0.0000229194,0.00003593277,0.0001042755,0.00009397849,0.00007348707],"domain_scores_gemma":[0.9989673,0.00006034936,0.00036559242,0.000100391226,0.00019164798,0.0003148095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045482488,0.0005108044,0.00048133323,0.0063861357,0.0005151559,0.00078612874,0.00057079206,0.00043119866,0.013010886],"category_scores_gemma":[0.00081124494,0.0002104817,0.00030317451,0.006363003,0.00019428093,0.00049274636,0.0009449481,0.00028188567,0.006734452],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017168942,0.0000827414,0.8484861,0.00049631135,0.00012579407,0.00013171884,0.00027211246,0.00018368328,0.0020478468,0.00052845397,0.108285174,0.039188385],"study_design_scores_gemma":[0.000014409823,0.000012379918,0.98541117,0.000025570062,0.000014166896,0.00005031149,0.000055478075,0.000065906854,0.00007200158,0.00003040603,0.014245402,0.000002851427],"about_ca_topic_score_codex":0.048013948,"about_ca_topic_score_gemma":0.04174422,"teacher_disagreement_score":0.048013948,"about_ca_system_score_codex":0.00067055883,"about_ca_system_score_gemma":0.00056681625,"threshold_uncertainty_score":0.09546894},"labels":[],"label_agreement":null},{"id":"W2514591177","doi":"10.3847/0004-637x/831/2/193","title":"A SEARCH FOR VERY HIGH ENERGY GAMMA RAYS FROM THE MISSING LINK BINARY PULSAR J1023+0038 WITH VERITAS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Pulsar; Astrophysics; Gamma ray; Millisecond pulsar; Neutron star; Astronomy","score_opus":0.016497770828373642,"score_gpt":0.22858451102767594,"score_spread":0.2120867401993023,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2514591177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99842083,0.00007330254,0.00016462193,0.000033179036,0.0000050475824,0.0000052116798,0.00025275984,0.000022637729,0.0010223666],"genre_scores_gemma":[0.9975897,0.000023817007,0.0007996681,0.00002486692,0.000008611319,0.0000041948883,0.0009998849,0.000007981297,0.00054135267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996624,0.000027028938,0.000017803332,0.0000947694,0.00011624874,0.00008188423],"domain_scores_gemma":[0.99913883,0.00014088125,0.00034513883,0.00011981079,0.00008080568,0.0001744752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056532415,0.0002544772,0.00025666924,0.0011786642,0.0004982516,0.000701538,0.0005583849,0.0004274252,0.0024395683],"category_scores_gemma":[0.00083724316,0.00028643405,0.00023271855,0.0008226337,0.00026443318,0.00030087726,0.0007653127,0.00035066737,0.00045276905],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011250364,0.00017906853,0.766375,0.00006732166,0.000108371874,0.0025757449,0.00048759856,0.0005525081,0.20650984,0.00057633454,0.0006221869,0.020821027],"study_design_scores_gemma":[0.000057681867,0.00043493105,0.9789717,0.000018917097,0.000059357862,0.0024770603,0.00032042872,0.0016156211,0.012940585,0.00019199,0.0028986211,0.000012997069],"about_ca_topic_score_codex":0.0026611013,"about_ca_topic_score_gemma":0.004487057,"teacher_disagreement_score":0.0026611013,"about_ca_system_score_codex":0.0003777319,"about_ca_system_score_gemma":0.00029836808,"threshold_uncertainty_score":0.008161128},"labels":[],"label_agreement":null},{"id":"W2514711714","doi":"10.3847/1538-4357/833/1/67","title":"ALMA SPECTROSCOPIC SURVEY IN THE HUBBLE ULTRA DEEP FIELD: SURVEY DESCRIPTION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":241,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Deutsche Forschungsgemeinschaft; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Redshift; Emission spectrum; Line (geometry); Hubble Deep Field; Spectral line; Hubble Ultra-Deep Field; Observational cosmology","score_opus":0.017927762141739714,"score_gpt":0.23215871150227047,"score_spread":0.21423094936053075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2514711714","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4392007,0.0017378388,0.022453358,0.00078656385,0.00006093341,0.0016549611,0.5065553,0.0013421789,0.02620816],"genre_scores_gemma":[0.59132457,0.0019015864,0.04390818,0.0008532277,0.00019151185,0.0029285655,0.34418195,0.00019838469,0.014511989],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995499,0.00008058353,0.00004602208,0.000110434084,0.00012654532,0.00008648007],"domain_scores_gemma":[0.9988047,0.00011571648,0.0003329961,0.00020743982,0.00033886544,0.00020021987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067726907,0.00036639287,0.00019490882,0.0036113143,0.0003041803,0.00054902944,0.000593198,0.00027295682,0.005701624],"category_scores_gemma":[0.0013547036,0.00012648881,0.00019024363,0.0036089898,0.00015275273,0.00047212167,0.00061529444,0.00021231589,0.0025153905],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016654121,0.00015132777,0.81053716,0.00041576524,0.000078466794,0.00014000002,0.00029651463,0.0028201318,0.0090314,0.0030156155,0.0641279,0.10921918],"study_design_scores_gemma":[0.000018398334,0.000053551677,0.9326301,0.0000412709,0.000014287182,0.00014262658,0.00013738494,0.0018895323,0.0011769752,0.00045470466,0.063421294,0.000019892015],"about_ca_topic_score_codex":0.021748343,"about_ca_topic_score_gemma":0.02384743,"teacher_disagreement_score":0.021748343,"about_ca_system_score_codex":0.0007338193,"about_ca_system_score_gemma":0.00066398236,"threshold_uncertainty_score":0.043243468},"labels":[],"label_agreement":null},{"id":"W2515230947","doi":"10.3847/1538-4357/834/2/137","title":"TIMING OF 29 PULSARS DISCOVERED IN THE PALFA SURVEY","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Office of Naval Research; National Aeronautics and Space Administration; Canada Research Chairs; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Science Foundation","keywords":"Pulsar; Observatory; Supernova; Millisecond pulsar; Binary pulsar; Neutron star; Interstellar medium; Rotation period","score_opus":0.04253436955992987,"score_gpt":0.36843235802062047,"score_spread":0.3258979884606906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2515230947","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99589926,0.00014392134,0.00024877934,0.000056975725,0.000012454563,0.000013669559,0.0012887031,0.000053201813,0.0022831047],"genre_scores_gemma":[0.9937184,0.00012756539,0.00044239906,0.00003935173,0.000020923319,0.000021565273,0.004266082,0.000009408455,0.0013541951],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976975,0.00002591552,0.000016264232,0.000060925788,0.0000683814,0.000058853006],"domain_scores_gemma":[0.9991061,0.00010071418,0.00030680592,0.000066543,0.0002618438,0.00015806712],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002888093,0.00016901626,0.00016707998,0.0016742448,0.0004057805,0.00051195646,0.00026701193,0.0001985426,0.0015518432],"category_scores_gemma":[0.00072316575,0.00009830391,0.00013689556,0.00088568626,0.00019177732,0.00022276718,0.00054935477,0.0002240715,0.0005123353],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017700993,0.000046631703,0.9668178,0.000034437817,0.000038709913,0.00050641486,0.00038556775,0.00010082088,0.008681979,0.00012125337,0.0011154374,0.021974038],"study_design_scores_gemma":[0.00000436911,0.00004527738,0.9958703,0.000004729214,0.000006800054,0.00019149274,0.00012436368,0.0001242007,0.00056689227,0.000013316323,0.0030449382,0.000003283043],"about_ca_topic_score_codex":0.0063368133,"about_ca_topic_score_gemma":0.015230609,"teacher_disagreement_score":0.0063368133,"about_ca_system_score_codex":0.0004349569,"about_ca_system_score_gemma":0.00027553827,"threshold_uncertainty_score":0.012599826},"labels":[],"label_agreement":null},{"id":"W2517147363","doi":"10.3847/0004-637x/830/2/126","title":"THE CARINA PROJECT. X. ON THE KINEMATICS OF OLD AND INTERMEDIATE-AGE STELLAR POPULATIONS*†","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Milky Way; Dwarf galaxy; Galaxy; Stars; Velocity dispersion; Local Group; Dwarf spheroidal galaxy; Irregular galaxy","score_opus":0.01599820542316196,"score_gpt":0.23371101146277196,"score_spread":0.21771280603961,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2517147363","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.71055186,0.014321004,0.04140869,0.0025167412,0.0005357961,0.0006976798,0.10656386,0.013586237,0.10981819],"genre_scores_gemma":[0.7974722,0.0017083646,0.057445254,0.00039780108,0.00022049631,0.0004827012,0.114367336,0.0028928837,0.025013035],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99952567,0.00012721732,0.00000963871,0.00016533319,0.00008952787,0.00008262361],"domain_scores_gemma":[0.99898356,0.00012464507,0.00016136933,0.00023250972,0.00023440461,0.00026349592],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001866934,0.0011250837,0.0003575842,0.0016024695,0.0005978839,0.0015111623,0.0008080844,0.00052296603,0.0050901235],"category_scores_gemma":[0.0010809972,0.00029724912,0.0004205786,0.0007893554,0.00029248223,0.00068313675,0.0017726161,0.0003040513,0.0036185156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0032651927,0.00038437673,0.43532154,0.0009863504,0.00051014626,0.00058101676,0.0018228482,0.014649749,0.01589807,0.020188052,0.098852836,0.40753976],"study_design_scores_gemma":[0.00043759603,0.0005239192,0.40611574,0.00051899767,0.00034884887,0.0006995523,0.0008148675,0.060187608,0.017700473,0.0076221074,0.50491804,0.000112337926],"about_ca_topic_score_codex":0.017940989,"about_ca_topic_score_gemma":0.016003447,"teacher_disagreement_score":0.017940989,"about_ca_system_score_codex":0.0007137501,"about_ca_system_score_gemma":0.00084028457,"threshold_uncertainty_score":0.03567314},"labels":[],"label_agreement":null},{"id":"W2517310700","doi":"10.3847/0004-637x/831/2/150","title":"EINSTEIN@HOME DISCOVERY OF A DOUBLE NEUTRON STAR BINARY IN THE PALFA SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Office of Naval Research; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Max-Planck-Gesellschaft; Natural Sciences and Engineering Research Council of Canada; European Commission; National Science Foundation; Compute Canada; McGill University; Canada Research Chairs; National Aeronautics and Space Administration; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association","keywords":"Neutron star; Pulsar; Binary pulsar; Gravitational wave; Eccentricity (behavior); Supernova; Millisecond pulsar; Orbital elements; Binary star","score_opus":0.021663958084546523,"score_gpt":0.3091930377975764,"score_spread":0.2875290797130299,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2517310700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98985773,0.00026158532,0.0003744097,0.00076444173,0.000046163612,0.00001456984,0.000522186,0.000050997056,0.00810797],"genre_scores_gemma":[0.9970906,0.00020385755,0.00043753898,0.00025658723,0.000051706767,0.0000059415756,0.0005388855,0.000010415347,0.0014044282],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998223,0.000021217213,0.000008910714,0.000047894137,0.00005593436,0.000043788434],"domain_scores_gemma":[0.9992669,0.00006789672,0.00020246512,0.00008575185,0.00013714455,0.00023981018],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003131232,0.00019987562,0.00013357747,0.0012574423,0.0005593179,0.0005733313,0.00025381352,0.00033527307,0.0028798648],"category_scores_gemma":[0.00070136954,0.000115865194,0.0001102586,0.0004904849,0.0003804158,0.0002492848,0.0008139687,0.00036429943,0.0005501379],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026933802,0.00008847739,0.9294149,0.00004590085,0.00005655299,0.010786908,0.0011368585,0.000043660024,0.011243754,0.0010454048,0.0052654753,0.040602755],"study_design_scores_gemma":[0.000028084638,0.00016705273,0.9489104,0.000029808594,0.000032600507,0.01380755,0.0006618961,0.00017693688,0.0030448206,0.00026698387,0.032858137,0.00001583195],"about_ca_topic_score_codex":0.006136908,"about_ca_topic_score_gemma":0.009778246,"teacher_disagreement_score":0.006136908,"about_ca_system_score_codex":0.00049153983,"about_ca_system_score_gemma":0.00026517466,"threshold_uncertainty_score":0.0122023225},"labels":[],"label_agreement":null},{"id":"W2517317009","doi":"10.3847/0004-637x/831/1/89","title":"A NEW γ-RAY LOUD, ECLIPSING LOW-MASS X-RAY BINARY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Light curve; Telescope; Photometry (optics); Binary number; Eclipse; Binary star; Luminosity; Neutron star; Accretion (finance)","score_opus":0.011944547550029931,"score_gpt":0.22792779038466948,"score_spread":0.21598324283463954,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2517317009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997426,0.00028823788,0.00031499867,0.00019132985,0.000039462255,0.000007754078,0.00006006399,0.000019699493,0.0016525241],"genre_scores_gemma":[0.99812955,0.000060656108,0.000328191,0.00021242251,0.000050982522,0.0000044951794,0.00017912318,0.000005801709,0.0010288028],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986553,0.000011092496,0.000012127938,0.00003797269,0.000025789792,0.00004747655],"domain_scores_gemma":[0.9997491,0.000033777793,0.00005947384,0.000030151374,0.000022013803,0.0001054816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001586884,0.00019588956,0.00033013604,0.00076116004,0.001355924,0.0009946475,0.00044447338,0.0008384523,0.0025271622],"category_scores_gemma":[0.000518123,0.00014388387,0.00012927101,0.0003239861,0.0005390268,0.0004258604,0.0006186243,0.00067716104,0.0008684546],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074145105,0.0012220027,0.7712134,0.00008675111,0.00005532847,0.0965029,0.0021472017,0.00022048342,0.07745041,0.004376759,0.0034602247,0.042523123],"study_design_scores_gemma":[0.00015019259,0.0014931662,0.7246762,0.00005659019,0.00006630042,0.23629889,0.0012794989,0.001405313,0.008704846,0.0026581734,0.023167772,0.000043126667],"about_ca_topic_score_codex":0.0012590297,"about_ca_topic_score_gemma":0.0017609786,"teacher_disagreement_score":0.0025271622,"about_ca_system_score_codex":0.00036103255,"about_ca_system_score_gemma":0.00021075421,"threshold_uncertainty_score":0.008454144},"labels":[],"label_agreement":null},{"id":"W2517690209","doi":"10.3847/0004-637x/831/1/113","title":"VERY HIGH ENERGY OBSERVATIONS OF THE BINARIES V 404 CYG AND 4U 0115+634 DURING GIANT X-RAY OUTBURSTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Luminosity; Flux (metallurgy); Eddington luminosity; Observatory; High energy; X-ray binary; Binary number","score_opus":0.011079713098652017,"score_gpt":0.19459291480272964,"score_spread":0.18351320170407762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2517690209","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980111,0.0000837078,0.00007213765,0.000022199467,0.000004000557,0.0000036550205,0.00016786618,0.000014066848,0.0016211828],"genre_scores_gemma":[0.9989711,0.000052607138,0.00013259986,0.0000130732515,0.0000060152015,0.0000043512955,0.00034568267,0.0000052433556,0.00046935386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999037,0.000009129242,0.0000058573537,0.000021465232,0.000027573473,0.00003238694],"domain_scores_gemma":[0.99978787,0.000026570628,0.000089178146,0.000017733864,0.000015073017,0.00006369144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017893223,0.0001978719,0.00023243029,0.00083490054,0.0004995491,0.00049960363,0.00021590517,0.0003014179,0.0016110351],"category_scores_gemma":[0.000396503,0.0001601964,0.00012804799,0.0005687645,0.000314785,0.00022327283,0.0006784558,0.00022452167,0.00023271146],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005785775,0.00010051802,0.84450114,0.00006492419,0.00011936684,0.0012594126,0.000723971,0.0006645581,0.1342912,0.00072521967,0.0010276047,0.015943594],"study_design_scores_gemma":[0.00000666088,0.000042654257,0.99691224,0.000006290633,0.000009044147,0.00013211474,0.00010640063,0.00020859667,0.0016945525,0.00008627925,0.0007913206,0.000003804993],"about_ca_topic_score_codex":0.0058098375,"about_ca_topic_score_gemma":0.01602553,"teacher_disagreement_score":0.0058098375,"about_ca_system_score_codex":0.00045687667,"about_ca_system_score_gemma":0.00022264889,"threshold_uncertainty_score":0.011552036},"labels":[],"label_agreement":null},{"id":"W2518326765","doi":"10.3847/0004-637x/832/1/50","title":"BANYAN. VIII. NEW LOW-MASS STARS AND BROWN DWARFS WITH CANDIDATE CIRCUMSTELLAR DISKS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"Brown dwarf; Circumstellar disk; Stars; Circumstellar dust; Stellar classification; Infrared","score_opus":0.006495742410252215,"score_gpt":0.20933200984186456,"score_spread":0.20283626743161234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2518326765","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99449843,0.0006026339,0.00028580276,0.000077164514,0.000011512943,0.000026400981,0.0006241727,0.00003225948,0.0038415603],"genre_scores_gemma":[0.9929696,0.00028309843,0.0009913443,0.000090657224,0.0000254914,0.000016000164,0.0028969003,0.000011855685,0.0027151152],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997286,0.000024952602,0.000017471135,0.00006502937,0.00009542915,0.00006845799],"domain_scores_gemma":[0.99947494,0.000071717695,0.0001567213,0.000042648844,0.000077002194,0.0001770499],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004554201,0.00033427542,0.00039238425,0.0014534094,0.0009989329,0.00093813165,0.00037051903,0.00025715865,0.0029069795],"category_scores_gemma":[0.00041348752,0.0001482224,0.00026502935,0.0011614314,0.00022240703,0.00030903317,0.0007516462,0.00028849283,0.00082844973],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028255783,0.00017889781,0.95416737,0.000094722316,0.0000477924,0.0014644552,0.0004355874,0.00012140278,0.01664567,0.00026690649,0.0008834848,0.025411315],"study_design_scores_gemma":[0.000011235216,0.00006778198,0.98825574,0.000013644697,0.00003103439,0.0014322832,0.00036796634,0.00029114893,0.0038906753,0.00010763392,0.005524356,0.0000065719564],"about_ca_topic_score_codex":0.006862579,"about_ca_topic_score_gemma":0.009972533,"teacher_disagreement_score":0.006862579,"about_ca_system_score_codex":0.00047136802,"about_ca_system_score_gemma":0.000489778,"threshold_uncertainty_score":0.013645291},"labels":[],"label_agreement":null},{"id":"W2518496494","doi":"10.3847/0004-637x/829/2/108","title":"BAYESIAN MASS ESTIMATES OF THE MILKY WAY: THE DARK AND LIGHT SIDES OF PARAMETER ASSUMPTIONS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Milky Way; Bayesian probability; Physics; Dark matter; Astrophysics; Mathematics; Statistics; Galaxy","score_opus":0.010079729558653923,"score_gpt":0.22309334456805918,"score_spread":0.21301361500940527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2518496494","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8146969,0.0011176987,0.17720215,0.00091717264,0.00001630606,0.00004394867,0.0004763598,0.00020209429,0.0053274343],"genre_scores_gemma":[0.9881422,0.00016089315,0.010929347,0.00010239601,0.000020743062,0.000017487277,0.00026007745,0.000024414418,0.0003423745],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99866045,0.00064247835,0.00006600753,0.00026602813,0.00027333753,0.00009173053],"domain_scores_gemma":[0.9821348,0.012710628,0.002166575,0.0015787608,0.0011508557,0.00025833293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0063974527,0.00044114148,0.00062828354,0.002120068,0.0004896893,0.002143599,0.0013423593,0.001038355,0.0017255092],"category_scores_gemma":[0.054670993,0.00038455668,0.00073637173,0.0007752133,0.0013933252,0.0026333267,0.0017432685,0.0009094293,0.00026759633],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071022473,0.000092137605,0.3859123,0.0002683276,0.00096463895,0.000514335,0.0016813391,0.2950986,0.00676097,0.18844308,0.002638874,0.11691521],"study_design_scores_gemma":[0.00014796876,0.00012370282,0.16145681,0.00032621887,0.00030003354,0.0005375548,0.0008588292,0.54525393,0.006319487,0.2791274,0.0053984947,0.00014959236],"about_ca_topic_score_codex":0.0062631443,"about_ca_topic_score_gemma":0.0035328032,"teacher_disagreement_score":0.0063974527,"about_ca_system_score_codex":0.0012092423,"about_ca_system_score_gemma":0.0005046276,"threshold_uncertainty_score":0.033833385},"labels":[],"label_agreement":null},{"id":"W2518605874","doi":"10.3847/1538-4357/833/1/31","title":"THE SHAPE OF THE INNER MILKY WAY HALO FROM OBSERVATIONS OF THE PAL 5 AND GD–1 STELLAR STREAMS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":172,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Halo; Flattening; Milky Way; Galactic halo; Gravitational potential; Galactic tide; STREAMS; Mass distribution; Galactic Center","score_opus":0.014643359639410042,"score_gpt":0.2053671365819735,"score_spread":0.19072377694256346,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2518605874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989594,0.000039935945,0.00026567237,0.000016589536,8.586873e-7,0.0000011653815,0.00013942685,0.000018195766,0.0005586919],"genre_scores_gemma":[0.9995734,0.00001711752,0.00012108628,0.0000050531007,0.0000012341703,6.844278e-7,0.00022659941,0.000004405418,0.00005035141],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999429,0.000009439305,0.000003229055,0.000016309019,0.000016826354,0.000011325698],"domain_scores_gemma":[0.99970704,0.00003776351,0.00009808402,0.00005438039,0.00004673117,0.000056043827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025491163,0.00014646591,0.0001682971,0.0005815831,0.0001758376,0.000591716,0.0002051917,0.00014621335,0.00057411625],"category_scores_gemma":[0.00088446646,0.0001556362,0.0003016893,0.00032546345,0.00019267084,0.00025088785,0.0006038731,0.00012072445,0.00017660481],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014863494,0.000011831718,0.9664089,0.000021537,0.00011496292,0.00008785533,0.00028376147,0.00665217,0.017714178,0.0006920135,0.00030482875,0.007559337],"study_design_scores_gemma":[0.0000079787005,0.000019571127,0.9865702,0.000007299052,0.000023061788,0.000043526205,0.00009491706,0.010979571,0.00136714,0.00025195998,0.00062734226,0.00000747739],"about_ca_topic_score_codex":0.007603243,"about_ca_topic_score_gemma":0.010552197,"teacher_disagreement_score":0.007603243,"about_ca_system_score_codex":0.00037705444,"about_ca_system_score_gemma":0.00018524694,"threshold_uncertainty_score":0.015117943},"labels":[],"label_agreement":null},{"id":"W2518636529","doi":"10.3847/0004-637x/827/2/153","title":"NONSINGULAR UNIVERSES IN GAUSS–BONNET GRAVITY’S RAINBOW","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Noncommutative and Quantum Gravity Theories","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Friedmann–Lemaître–Robertson–Walker metric; Cosmology; Physics; Gravitational singularity; Mathematical physics; Classical mechanics; Gauss–Bonnet gravity; Initial singularity; Singularity; Theoretical physics; Gravitation; Mathematical analysis; Astrophysics; Mathematics; Universe; Quantum mechanics; De Sitter universe","score_opus":0.009068380291484232,"score_gpt":0.24250087741692086,"score_spread":0.23343249712543662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2518636529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95300335,0.00024766306,0.017420806,0.0005903392,0.00008639358,0.000017617323,0.000024219318,0.00010725023,0.028502468],"genre_scores_gemma":[0.99533325,0.0000624607,0.0027173914,0.00008019997,0.000049563438,0.0000054453762,0.000019248158,0.000018806239,0.0017136198],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997701,0.00006846951,0.000009717749,0.0000328703,0.00006385877,0.000054925527],"domain_scores_gemma":[0.99947304,0.000076299126,0.00010453718,0.00013368366,0.00004834135,0.00016417158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007741931,0.00043915148,0.00067442155,0.00070961803,0.001111594,0.0009698572,0.00047825303,0.0008464927,0.002058486],"category_scores_gemma":[0.0010274026,0.0002963897,0.00076529663,0.00028860313,0.0030693905,0.002018258,0.0017607647,0.0013234427,0.00018506793],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031760384,0.000028209397,0.0006862956,0.000013829561,0.000013017504,0.00038005592,0.00024001737,0.0040896796,0.0028667983,0.9899114,0.00032633767,0.0014126447],"study_design_scores_gemma":[0.000046032448,0.00008399501,0.0033820518,0.000013459724,0.000011939061,0.0005303411,0.00021427657,0.03731053,0.0010778331,0.9553505,0.0019476742,0.000031254738],"about_ca_topic_score_codex":0.0011538228,"about_ca_topic_score_gemma":0.0010502982,"teacher_disagreement_score":0.002058486,"about_ca_system_score_codex":0.0007039091,"about_ca_system_score_gemma":0.00044888433,"threshold_uncertainty_score":0.0068863034},"labels":[],"label_agreement":null},{"id":"W2520426733","doi":"10.3847/0004-637x/831/2/177","title":"MagAO IMAGING OF LONG-PERIOD OBJECTS (MILO). II. A PUZZLING WHITE DWARF AROUND THE SUN-LIKE STAR HD 11112","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"White dwarf; Spectral energy distribution; Circumbinary planet; Radial velocity; Binary star; Binary number; Black dwarf; Primary (astronomy); Stars","score_opus":0.009298034669668527,"score_gpt":0.2192542019630217,"score_spread":0.20995616729335317,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2520426733","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949169,0.000103491584,0.0012008622,0.00007898463,0.0000058136425,0.0000057743227,0.00023071325,0.000106021515,0.0033514441],"genre_scores_gemma":[0.9970409,0.00002211427,0.0021711376,0.000016447824,0.000005160948,0.000002578544,0.00019168382,0.000009843066,0.0005401004],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996126,0.0000030199546,0.0000015153315,0.0000133535295,0.000010022805,0.000010827258],"domain_scores_gemma":[0.9998596,0.000021948501,0.000033811502,0.000015615557,0.000021275082,0.00004781391],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001406309,0.00010466907,0.00011761161,0.0005247811,0.00031084928,0.0002797481,0.0001833636,0.0002576996,0.0011609812],"category_scores_gemma":[0.0002634658,0.00012941124,0.00013560455,0.00020198013,0.00012797183,0.00015429466,0.0002349106,0.00016789639,0.00017938731],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004970639,0.00019358881,0.41636658,0.0001259059,0.000106342384,0.0011940893,0.0005844365,0.004309094,0.5336325,0.002055787,0.0018497786,0.03908478],"study_design_scores_gemma":[0.000025492653,0.00015552904,0.95792186,0.000015714002,0.000051461233,0.0011095995,0.00019585091,0.018850626,0.018483901,0.0007247269,0.0024508333,0.000014401648],"about_ca_topic_score_codex":0.0016706954,"about_ca_topic_score_gemma":0.00597572,"teacher_disagreement_score":0.0016706954,"about_ca_system_score_codex":0.00029149288,"about_ca_system_score_gemma":0.000098037686,"threshold_uncertainty_score":0.0038838387},"labels":[],"label_agreement":null},{"id":"W2521069020","doi":"10.3847/0004-637x/830/2/130","title":"THE IMPLICIT CONTRIBUTION OF SLAB MODES TO THE PERPENDICULAR DIFFUSION COEFFICIENT OF PARTICLES INTERACTING WITH TWO-COMPONENT TURBULENCE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Slab; Perpendicular; Magnetic field; Superposition principle; Diffusion; Turbulence; Field (mathematics); Shock (circulatory)","score_opus":0.0042917897667908616,"score_gpt":0.22631102813083287,"score_spread":0.222019238364042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2521069020","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95119274,0.00033997666,0.042159643,0.00036782963,0.000076185665,0.000035862606,0.00004484502,0.0001104408,0.0056724628],"genre_scores_gemma":[0.99613035,0.00012877745,0.002594516,0.00001957115,0.000023005205,0.000016547823,0.000020231244,0.000023757297,0.001043208],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998578,0.000051506264,0.000006618674,0.0000139549775,0.00002660951,0.000043534736],"domain_scores_gemma":[0.9993375,0.0002970705,0.00010054104,0.00006000752,0.00009806927,0.0001068629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000416909,0.00081131957,0.0005878645,0.0004882968,0.0006144974,0.0011151169,0.00069024315,0.00072321366,0.0012481605],"category_scores_gemma":[0.0015059435,0.0003203099,0.000510838,0.00032687397,0.001267522,0.001122407,0.0011563011,0.00086592406,0.00011421416],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005137829,0.0003486326,0.005420063,0.00018438011,0.00010606594,0.00092587294,0.00036984167,0.80633503,0.09075145,0.08865065,0.0006989506,0.0056953924],"study_design_scores_gemma":[0.000021026315,0.000025193565,0.0005155461,0.0000035246035,0.000008299483,0.000019639696,0.000018416122,0.99584275,0.0014276225,0.002020017,0.000083414634,0.000014574147],"about_ca_topic_score_codex":0.0064629167,"about_ca_topic_score_gemma":0.0019467664,"teacher_disagreement_score":0.0064629167,"about_ca_system_score_codex":0.0005134952,"about_ca_system_score_gemma":0.0006409605,"threshold_uncertainty_score":0.012850642},"labels":[],"label_agreement":null},{"id":"W2521412154","doi":"10.3847/1538-4357/833/2/226","title":"THE GALEX TIME DOMAIN SURVEY. II. WAVELENGTH-DEPENDENT VARIABILITY OF ACTIVE GALACTIC NUCLEI IN THE PAN-STARRS1 MEDIUM DEEP SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Accretion (finance); Spectral index; Flux (metallurgy); Amplitude; Active galactic nucleus; Lambda; Spectral line; Wavelength; Astronomy; Galaxy","score_opus":0.013952999883746412,"score_gpt":0.23520996719738815,"score_spread":0.22125696731364175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2521412154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947179,0.00006107414,0.0002755715,0.000023310997,0.0000020807736,0.000007037609,0.0040794252,0.000027546706,0.0008061014],"genre_scores_gemma":[0.98572505,0.00006781064,0.0006860562,0.000025204647,0.0000076104943,0.000017904636,0.012658828,0.000016663354,0.00079482386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998153,0.000040375842,0.000012888255,0.00005553755,0.00003798121,0.000037963975],"domain_scores_gemma":[0.9991122,0.00012908057,0.00040555405,0.00013266792,0.000090330876,0.00013019747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034645223,0.00021404526,0.00012282944,0.0012419204,0.00012836217,0.00036026037,0.00027720517,0.00016248738,0.0008350879],"category_scores_gemma":[0.00076623436,0.000082785744,0.00022407941,0.00074688473,0.00013795792,0.00023225792,0.0006258759,0.00015023297,0.000447269],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014762433,0.000024401528,0.98600465,0.00001767721,0.000058851412,0.00006953503,0.00011591986,0.000720344,0.003770079,0.0001435905,0.00089794496,0.008029542],"study_design_scores_gemma":[0.0000025834538,0.000011447614,0.99825567,0.000001331452,0.000004417727,0.00006918724,0.000037748483,0.00037457436,0.0003359766,0.000013233738,0.0008921727,0.0000017181602],"about_ca_topic_score_codex":0.0045455787,"about_ca_topic_score_gemma":0.006323524,"teacher_disagreement_score":0.0045455787,"about_ca_system_score_codex":0.00022726927,"about_ca_system_score_gemma":0.000076820164,"threshold_uncertainty_score":0.00903821},"labels":[],"label_agreement":null},{"id":"W2521959911","doi":"10.3847/0004-637x/832/2/145","title":"AGE DEPENDENCE OF WIND PROPERTIES FOR SOLAR-TYPE STARS: A 3D STUDY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Stars; Angular momentum; Magnetohydrodynamics; Solar wind; Interplanetary spaceflight; Stellar rotation; RADIUS; Doppler effect; Stellar magnetic field","score_opus":0.025542128118582086,"score_gpt":0.24267637338390755,"score_spread":0.21713424526532546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2521959911","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963989,0.00009000185,0.0018354502,0.00003940974,0.000008929672,0.000009321846,0.00066338084,0.0000770074,0.00087768765],"genre_scores_gemma":[0.99790406,0.000071503295,0.0010989569,0.000009906135,0.000006408961,0.0000058363494,0.00070143346,0.000021207974,0.00018075634],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99992025,0.000014033564,0.000006295009,0.00002162221,0.000016362352,0.000021451775],"domain_scores_gemma":[0.99963784,0.00010441063,0.000060550883,0.000051348696,0.000055447945,0.00009043531],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023532085,0.00039810094,0.00039057297,0.00071632385,0.0003370463,0.00073605665,0.0003963329,0.00074710115,0.0010902949],"category_scores_gemma":[0.0006107527,0.00027075136,0.0009701193,0.0005047811,0.000276015,0.00034015134,0.00037665962,0.00039915487,0.00028982604],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031906544,0.0003058747,0.22733484,0.00006777906,0.00020269625,0.0008201283,0.00027894773,0.7445126,0.017809708,0.0012736141,0.00087776186,0.006196997],"study_design_scores_gemma":[0.000024083703,0.000055415687,0.07144149,0.0000075331227,0.000019988458,0.00013784553,0.00008661939,0.92583096,0.0013223161,0.00048153402,0.0005644497,0.000027820892],"about_ca_topic_score_codex":0.007587991,"about_ca_topic_score_gemma":0.004796974,"teacher_disagreement_score":0.007587991,"about_ca_system_score_codex":0.00032906546,"about_ca_system_score_gemma":0.00023772774,"threshold_uncertainty_score":0.015087664},"labels":[],"label_agreement":null},{"id":"W2522041221","doi":"10.1088/0004-637x/810/2/117","title":"A SPECTROSCOPIC ANALYSIS OF THE K0 III BINARY<i>ϵ</i>CYGNI","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Radial velocity; Line (geometry); Granulation; Amplitude; Stellar rotation; Rotation (mathematics); Electron temperature; Stars; Plasma; Optics","score_opus":0.014231283488538284,"score_gpt":0.23907084456706093,"score_spread":0.22483956107852265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2522041221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998137,0.00006631742,0.00012854583,0.000024128482,0.0000026067407,0.000012065039,0.0002912037,0.000012276946,0.0013257219],"genre_scores_gemma":[0.9975356,0.000058059948,0.0004334208,0.000027422755,0.0000058397604,0.000009103974,0.0013490741,0.000005374229,0.00057599833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999323,0.000003629634,0.000003501651,0.000020073257,0.00002050193,0.000020027384],"domain_scores_gemma":[0.9998191,0.000012420889,0.000057517853,0.000012823605,0.00004663045,0.00005148227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009733782,0.00022239261,0.00017463605,0.0010900311,0.0004038791,0.00029225086,0.00012468974,0.00015131223,0.0006862872],"category_scores_gemma":[0.00028244604,0.00009061323,0.00013751556,0.00080701703,0.00016759409,0.000119178716,0.00018738139,0.00012921999,0.00034751376],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007625861,0.00013405857,0.6242443,0.00006154788,0.000041033483,0.0009309549,0.0005206156,0.0004059277,0.34685668,0.00037377255,0.0010219733,0.02464652],"study_design_scores_gemma":[0.000002193934,0.000027795608,0.9974765,0.0000018381264,0.000005352578,0.00019866756,0.000029453024,0.00017171516,0.001529924,0.000015164125,0.00053976284,0.0000015939761],"about_ca_topic_score_codex":0.012519893,"about_ca_topic_score_gemma":0.013684348,"teacher_disagreement_score":0.012519893,"about_ca_system_score_codex":0.00066294346,"about_ca_system_score_gemma":0.00030194453,"threshold_uncertainty_score":0.024894059},"labels":[],"label_agreement":null},{"id":"W2522337348","doi":"10.3847/1538-4357/835/2/167","title":"Bayesian Mass Estimates of the Milky Way: Including Measurement Uncertainties with Hierarchical Bayes","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; McMaster University","funders":"","keywords":"Galaxy; Bayesian probability; Globular cluster; Physics; Milky Way; Bayes' theorem; Astrophysics; Satellite galaxy; Bayesian hierarchical modeling; Algorithm; Statistical physics; Statistics; Computer science; Mathematics","score_opus":0.01888366935050413,"score_gpt":0.2353086743077421,"score_spread":0.216425004957238,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2522337348","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.041888393,0.00061528565,0.95427424,0.00031419095,0.000018531973,0.000069176014,0.00027424013,0.0002367954,0.0023091142],"genre_scores_gemma":[0.72018695,0.0006095998,0.27505192,0.0002589081,0.00014435523,0.00018289658,0.001003553,0.00015758359,0.002404338],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99667895,0.0016707832,0.00014027316,0.00055609044,0.000763802,0.00018998208],"domain_scores_gemma":[0.98119307,0.0145455925,0.0014170368,0.0014580821,0.0011240172,0.00026219094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007993615,0.0008642508,0.0011701303,0.0027583567,0.0009677459,0.0021730948,0.0034688178,0.0012087056,0.0023614315],"category_scores_gemma":[0.04792759,0.0010013784,0.0011779773,0.001907299,0.0018302788,0.003525135,0.002163772,0.0017234161,0.0003671434],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013059918,0.00005954677,0.022862107,0.000143661,0.0003602762,0.00020842956,0.0004121297,0.70987207,0.0010138752,0.1690888,0.0024034786,0.093445025],"study_design_scores_gemma":[0.000024145573,0.000014719326,0.003944637,0.00005079729,0.000041599465,0.000053492666,0.000050330127,0.8375123,0.00041922778,0.15666258,0.0011900486,0.000036150002],"about_ca_topic_score_codex":0.031027677,"about_ca_topic_score_gemma":0.024428004,"teacher_disagreement_score":0.031027677,"about_ca_system_score_codex":0.002450636,"about_ca_system_score_gemma":0.0017375165,"threshold_uncertainty_score":0.061694145},"labels":[],"label_agreement":null},{"id":"W2522464319","doi":"10.3847/1538-4357/aa5df6","title":"DDO 216-A1: A Central Globular Cluster in a Low-luminosity Transition-type Galaxy<sup>∗</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Globular cluster; RR Lyrae variable; Distance modulus; Metallicity; Absolute magnitude; Surface brightness; RADIUS; Cluster (spacecraft); Horizontal branch; Brightest cluster galaxy","score_opus":0.010010341462456024,"score_gpt":0.22556803047805218,"score_spread":0.21555768901559616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2522464319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925438,0.00008565748,0.00030227008,0.00017486794,0.000032008473,0.000016316739,0.0019028734,0.00014669739,0.004795393],"genre_scores_gemma":[0.9911069,0.00005811277,0.0012954662,0.00007475468,0.000038449743,0.000009167161,0.004490744,0.000034931218,0.0028914735],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999429,0.0000019911834,0.000005236587,0.000020245845,0.000013909062,0.000015624364],"domain_scores_gemma":[0.99970955,0.000019625908,0.00005394195,0.000029455518,0.000023297122,0.00016408566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010133855,0.0001993317,0.00021486868,0.00067884644,0.0007725721,0.00052077085,0.00061085453,0.00038449562,0.005544751],"category_scores_gemma":[0.00030900727,0.00008047799,0.00016810463,0.00062991254,0.00033015778,0.00020518721,0.00047220968,0.00016915088,0.0028656854],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020228326,0.0004313911,0.7806198,0.00030728203,0.000055474928,0.01825683,0.0012899936,0.0019381577,0.11905625,0.0025121784,0.020120574,0.053389262],"study_design_scores_gemma":[0.0000447698,0.00028281272,0.9506383,0.000027607162,0.000031697018,0.0074705333,0.00083315274,0.0025153852,0.010917804,0.00075921946,0.026448326,0.000030395408],"about_ca_topic_score_codex":0.003259232,"about_ca_topic_score_gemma":0.0033702177,"teacher_disagreement_score":0.005544751,"about_ca_system_score_codex":0.00047996064,"about_ca_system_score_gemma":0.00012924045,"threshold_uncertainty_score":0.018549025},"labels":[],"label_agreement":null},{"id":"W2523032608","doi":"10.3847/0004-637x/829/1/44","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. XX. RedGOLD BACKGROUND GALAXY CLUSTER DETECTIONS","year":2016,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"Agence Nationale de la Recherche","keywords":"Physics; Virgo Cluster; Astrophysics; Galaxy cluster; Cluster (spacecraft); Galaxy; Redshift; Astronomy; Computer science","score_opus":0.06403681655411095,"score_gpt":0.30897119881690205,"score_spread":0.2449343822627911,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2523032608","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8284117,0.0012609484,0.012646147,0.000322446,0.00006544025,0.0002076829,0.12173802,0.0035199837,0.03182755],"genre_scores_gemma":[0.7556853,0.00038971283,0.023751535,0.00024598694,0.000042808744,0.00013505093,0.20853043,0.0005318864,0.010687266],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995839,0.000045265926,0.000013753068,0.00012147444,0.00015499804,0.00008067616],"domain_scores_gemma":[0.99954224,0.000042863227,0.00010074325,0.00013470976,0.00009784206,0.000081743165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062278315,0.0002288839,0.0001983551,0.002475518,0.00026781327,0.00069285167,0.0005647447,0.00018573669,0.004643371],"category_scores_gemma":[0.0009493013,0.0002056663,0.00025792673,0.0016353787,0.000099908306,0.00029624646,0.00063497515,0.00016203329,0.003113402],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024153707,0.000088044464,0.81134593,0.00015846327,0.0001388149,0.00020305293,0.00027119706,0.0026806784,0.006345991,0.0028569151,0.06688939,0.10877994],"study_design_scores_gemma":[0.000028926252,0.000029834535,0.9230758,0.000039421982,0.000037789996,0.00022523265,0.00010260088,0.007091712,0.0033529976,0.00069162174,0.065301806,0.00002233809],"about_ca_topic_score_codex":0.03466988,"about_ca_topic_score_gemma":0.06367787,"teacher_disagreement_score":0.03466988,"about_ca_system_score_codex":0.00057894335,"about_ca_system_score_gemma":0.00036515653,"threshold_uncertainty_score":0.06893617},"labels":[],"label_agreement":null},{"id":"W2523731583","doi":"10.3847/1538-4357/835/2/151","title":"All-sky Search for Time-integrated Neutrino Emission from Astrophysical Sources with 7 yr of IceCube Data","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":320,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; University of Oxford; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Neutrino; Sky; Angular resolution (graph drawing); Astrophysics; Neutrino detector; Point source; Flux (metallurgy); Muon neutrino; Astronomy; Muon; Neutrino astronomy; Event (particle physics); Astroparticle physics; Event reconstruction; Detector; Particle physics; Neutrino oscillation","score_opus":0.025565424211950186,"score_gpt":0.2753443604477234,"score_spread":0.24977893623577324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2523731583","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9801666,0.00039312014,0.0032075085,0.00009955762,0.000015852504,0.000032052638,0.011616859,0.00016233923,0.004306074],"genre_scores_gemma":[0.9345933,0.00039986538,0.013682519,0.00006466111,0.000038524475,0.00007348981,0.050031923,0.000088298184,0.001027341],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996823,0.00006503597,0.000016486145,0.00009358645,0.00007415557,0.00006852477],"domain_scores_gemma":[0.9994728,0.00014108204,0.00014146412,0.000080756705,0.00008489228,0.00007905665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00097147387,0.00030617855,0.00048503262,0.001277205,0.00033966947,0.00088615646,0.00040911717,0.00025713953,0.0012879218],"category_scores_gemma":[0.0009799929,0.00017745436,0.00047981992,0.0017093673,0.0002311747,0.0005136441,0.00070873805,0.000304579,0.00033699168],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011173517,0.00022685596,0.90191483,0.00018571006,0.0012126783,0.0006771008,0.00035655938,0.011885303,0.04119001,0.002509495,0.0057128044,0.033011336],"study_design_scores_gemma":[0.00007169776,0.00022685374,0.93693817,0.000052915544,0.00032139636,0.0005885434,0.00040544005,0.020058703,0.01818353,0.001945126,0.021165816,0.000041840645],"about_ca_topic_score_codex":0.005849972,"about_ca_topic_score_gemma":0.014485876,"teacher_disagreement_score":0.005849972,"about_ca_system_score_codex":0.00041142388,"about_ca_system_score_gemma":0.00077815866,"threshold_uncertainty_score":0.011631787},"labels":[],"label_agreement":null},{"id":"W2523756054","doi":"10.3847/1538-4357/aa6a19","title":"Late-time Cooling of Neutron Star Transients and the Physics of the Inner Crust","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Neutron star; Crust; Thermal; Thermal equilibrium; Inner core; Neutron; Accretion (finance); Cooling curve","score_opus":0.012692388602298387,"score_gpt":0.2267512227409642,"score_spread":0.21405883413866583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2523756054","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972596,0.00021296201,0.001121018,0.000023771918,0.0000027674662,0.000004521965,0.000095731426,0.000056829984,0.0012227782],"genre_scores_gemma":[0.99958736,0.00003886048,0.00016887648,0.000003900716,9.571266e-7,0.0000017247004,0.00006118588,0.000008661862,0.00012845117],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999962,0.000003826944,0.0000024490548,0.000013426006,0.0000075417065,0.000010738418],"domain_scores_gemma":[0.99984443,0.000026770094,0.00006021256,0.000022143253,0.000021128857,0.000025340027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018810351,0.00030027435,0.00023985466,0.00032962972,0.0002616327,0.00037461793,0.00032539832,0.00016741887,0.0012698664],"category_scores_gemma":[0.00039628326,0.0001719679,0.00030630818,0.00018580577,0.00032300138,0.00037278977,0.00029793856,0.0003008655,0.0001413182],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040078326,0.00004571324,0.14632742,0.00012766838,0.00007464578,0.0005906248,0.0002843344,0.032752465,0.80908483,0.0035738703,0.0001743526,0.0065632965],"study_design_scores_gemma":[0.00004959452,0.00020182517,0.71839434,0.000021473394,0.00004401074,0.00034833822,0.00016114693,0.15257356,0.12528394,0.001400708,0.0014838651,0.000037172398],"about_ca_topic_score_codex":0.0037018426,"about_ca_topic_score_gemma":0.0018482307,"teacher_disagreement_score":0.0037018426,"about_ca_system_score_codex":0.00066221476,"about_ca_system_score_gemma":0.0001449012,"threshold_uncertainty_score":0.0073605776},"labels":[],"label_agreement":null},{"id":"W2524538378","doi":"10.3847/0004-637x/832/1/62","title":"DISCOVERY OF A POSSIBLE COOL WHITE DWARF COMPANION FROM THE AllWISE MOTION SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"White dwarf; Physics; Astrophysics; Proper motion; Flux (metallurgy); Spectral line; Spectroscopy; White (mutation); Infrared; Orbital motion; Near-infrared spectroscopy; Astronomy; Stars; Chemistry; Optics","score_opus":0.016610889737592827,"score_gpt":0.22677283776229132,"score_spread":0.21016194802469848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2524538378","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985763,0.000112536734,0.00028496204,0.00004887098,0.000015284217,0.0000033488564,0.000093122,0.000019737678,0.0008458931],"genre_scores_gemma":[0.99880505,0.00004713361,0.00038199546,0.0000540238,0.000019933259,0.000002279542,0.00028113712,0.0000074766763,0.00040096208],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985063,0.000010851137,0.000010176137,0.00004498666,0.000043238335,0.000040148036],"domain_scores_gemma":[0.9994024,0.000031385505,0.00018860347,0.00006830427,0.00007854316,0.0002307845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028691316,0.00025847618,0.0003258357,0.0010560512,0.00084454304,0.0006484526,0.0002859159,0.00035528635,0.0010378126],"category_scores_gemma":[0.00041835,0.00018342357,0.00017034229,0.0005786182,0.00030886737,0.00036582586,0.0010882916,0.00031855152,0.00047116497],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012935407,0.0001036915,0.91571695,0.0000291519,0.000046098736,0.0017622722,0.0010220514,0.00007304421,0.06261521,0.0005892217,0.0011153049,0.016797703],"study_design_scores_gemma":[0.0000072670578,0.00014819221,0.9870508,0.000009766946,0.000025175466,0.0018064522,0.00041214726,0.0003326369,0.0033091975,0.00017506797,0.0067155836,0.000007860066],"about_ca_topic_score_codex":0.0017983152,"about_ca_topic_score_gemma":0.004807179,"teacher_disagreement_score":0.0017983152,"about_ca_system_score_codex":0.00021855274,"about_ca_system_score_gemma":0.00020314244,"threshold_uncertainty_score":0.0035757422},"labels":[],"label_agreement":null},{"id":"W2524764669","doi":"10.3847/0004-637x/832/2/187","title":"THE MASSIVE PROTOSTELLAR CLUSTER NGC 6334I AT 220 au RESOLUTION: DISCOVERY OF FURTHER MULTIPLICITY, DIVERSITY, AND A HOT MULTI-CORE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Submillimeter Array; Outflow; Millimeter; Maser; RADIUS; Bipolar outflow; Brightness; Brightness temperature; Protostar; Luminosity","score_opus":0.020677999956046883,"score_gpt":0.24018280831157723,"score_spread":0.21950480835553035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2524764669","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989188,0.00008228776,0.00031344706,0.000022589094,0.0000018572239,0.000002358516,0.000081204074,0.000032377353,0.0005451555],"genre_scores_gemma":[0.99902475,0.000015159358,0.00062435376,0.000015695943,0.0000035663513,0.000002817753,0.00016145989,0.0000046310656,0.00014754293],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991643,0.000004412594,0.0000024713115,0.00002582874,0.000027957825,0.000022796241],"domain_scores_gemma":[0.9998196,0.000016658665,0.000043674125,0.000024409968,0.000021843529,0.00007392658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009274116,0.0001428986,0.00019573496,0.0005460672,0.0004346282,0.00038398738,0.0003026146,0.00022958375,0.000808268],"category_scores_gemma":[0.00024063505,0.00015769439,0.00014041716,0.0003637981,0.0002205275,0.00017096633,0.00057088025,0.00028778188,0.00015647693],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033688673,0.000070844704,0.5068276,0.000044897886,0.0001230063,0.0009023083,0.0008645274,0.0011411043,0.46914485,0.00077110325,0.0015608267,0.018212073],"study_design_scores_gemma":[0.000008529547,0.000026673259,0.9925889,0.000004167317,0.000018310962,0.00031222808,0.00012071482,0.001638065,0.0040321,0.00017036057,0.0010721077,0.000007879819],"about_ca_topic_score_codex":0.004459717,"about_ca_topic_score_gemma":0.011361248,"teacher_disagreement_score":0.004459717,"about_ca_system_score_codex":0.00029413713,"about_ca_system_score_gemma":0.0001163225,"threshold_uncertainty_score":0.008867502},"labels":[],"label_agreement":null},{"id":"W2524770893","doi":"10.3847/1538-4357/834/2/149","title":"THE EVOLUTION OF GAS GIANT ENTROPY DURING FORMATION BY RUNAWAY ACCRETION","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Planet; Radiative transfer; Accretion (finance); Opacity; Effective temperature; Radiative cooling; Giant planet; Entropy (arrow of time); Thermodynamics; Planetary system; Stars; Quantum mechanics","score_opus":0.006403236868412289,"score_gpt":0.2271381417910652,"score_spread":0.2207349049226529,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2524770893","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981862,0.000049421185,0.00070460496,0.00003285505,0.0000037719208,0.0000029185278,0.00012424272,0.000049250113,0.00084665633],"genre_scores_gemma":[0.99933344,0.000017521848,0.00034086083,0.0000053947297,0.0000015116644,0.0000036020504,0.0001238166,0.000017776643,0.00015590314],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999118,0.000020156538,0.000003621811,0.00001901378,0.000016646021,0.00002872219],"domain_scores_gemma":[0.99940467,0.0002827184,0.00011022624,0.000056039647,0.000057536632,0.00008887395],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003104403,0.0005033476,0.00034441505,0.0005514393,0.00039303344,0.00088911917,0.0005962595,0.0007261874,0.001133345],"category_scores_gemma":[0.0024165658,0.00031268052,0.0006056161,0.00036131009,0.0007015704,0.00063722464,0.0006334822,0.00049108063,0.0001533837],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016248084,0.00004232628,0.044943612,0.000033943827,0.00009461249,0.000312066,0.00009786245,0.9450547,0.00515372,0.0019123437,0.00019880741,0.0019936133],"study_design_scores_gemma":[0.000035920788,0.00009342199,0.02387927,0.0000118050575,0.000030263138,0.00008139386,0.000057118014,0.9711879,0.003188299,0.0010720199,0.00033855846,0.000024011544],"about_ca_topic_score_codex":0.0070196483,"about_ca_topic_score_gemma":0.0035986926,"teacher_disagreement_score":0.0070196483,"about_ca_system_score_codex":0.00089562073,"about_ca_system_score_gemma":0.00040182332,"threshold_uncertainty_score":0.01395756},"labels":[],"label_agreement":null},{"id":"W2526277165","doi":"10.3847/0004-637x/832/2/114","title":"SPT0346-52: NEGLIGIBLE AGN ACTIVITY IN A COMPACT, HYPER-STARBURST GALAXY AT z = 5.7","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Commonwealth Scientific and Industrial Research Organisation; Australian Government; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Active galactic nucleus; Luminosity; Luminous infrared galaxy; Infrared; Astronomy; Telescope","score_opus":0.010375929947266641,"score_gpt":0.22123307744360432,"score_spread":0.2108571474963377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2526277165","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978315,0.00007331316,0.00011191274,0.000022172178,0.0000059581494,0.000004090023,0.00032488044,0.00003549963,0.0015906076],"genre_scores_gemma":[0.9991967,0.000021561156,0.00008379053,0.000015513855,0.000005733655,0.0000015548568,0.00046559752,0.0000053869385,0.00020414677],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999841,0.000009180703,0.000008843702,0.000045124885,0.00004240255,0.00005348614],"domain_scores_gemma":[0.99949455,0.000015564783,0.00013034098,0.00004226305,0.00004776506,0.00026942298],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013842742,0.00024589503,0.00037907113,0.00050340296,0.00055901916,0.00072576024,0.0003025563,0.00029321318,0.002600238],"category_scores_gemma":[0.00029411216,0.00014791772,0.0002335018,0.00048071195,0.00033864158,0.0002485543,0.0005246031,0.00027424333,0.0009665867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068879116,0.00022047947,0.924426,0.000051516465,0.00008609253,0.0025913098,0.00036381232,0.00041135523,0.05959685,0.00035112887,0.0011432321,0.010069466],"study_design_scores_gemma":[0.000013181317,0.00016221071,0.9948791,0.0000042476445,0.000013273619,0.0017909786,0.00011923857,0.00038485727,0.0017139033,0.0000616732,0.00085333193,0.0000040734594],"about_ca_topic_score_codex":0.0043188385,"about_ca_topic_score_gemma":0.0045666536,"teacher_disagreement_score":0.0043188385,"about_ca_system_score_codex":0.00027034714,"about_ca_system_score_gemma":0.0001581603,"threshold_uncertainty_score":0.008698702},"labels":[],"label_agreement":null},{"id":"W2526698545","doi":"10.3847/1538-4357/aa73d4","title":"Accretion in Radiative Equipartition (AiRE) Disks","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Equipartition theorem; Physics; Accretion (finance); Astrophysics; Radiative transfer; Radiation pressure; Supermassive black hole; Accretion disc; Cosmic time; Radiation; Eddington luminosity; Instability; Radiative cooling; Mechanics; Active galactic nucleus; Star formation; Galaxy; Quantum mechanics; Magnetic field","score_opus":0.02398314616325856,"score_gpt":0.28048168765432374,"score_spread":0.25649854149106516,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2526698545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9723813,0.001823805,0.01679367,0.00015155945,0.00004370143,0.000025566122,0.000097836964,0.00017795096,0.008504623],"genre_scores_gemma":[0.9984479,0.0001423385,0.0009777619,0.000019210878,0.000029784513,0.000006243572,0.000027489303,0.000006523126,0.00034269394],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99971455,0.00007571845,0.000025920936,0.00008411088,0.000046477733,0.000053089567],"domain_scores_gemma":[0.99894065,0.00022896567,0.0004759928,0.00018579022,0.00006222921,0.00010633919],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034873272,0.00040770293,0.00045838233,0.00054458325,0.00048908265,0.0011639118,0.00085546693,0.000748409,0.00090249395],"category_scores_gemma":[0.0020460892,0.00026175473,0.00030606095,0.00026137242,0.0011808786,0.0013232846,0.0017529399,0.00039657482,0.00023976938],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092072634,0.0003236421,0.0907073,0.00061396154,0.00031650843,0.010105787,0.0015615878,0.21616322,0.3541539,0.26842064,0.0018614621,0.054851297],"study_design_scores_gemma":[0.00037987903,0.00064603944,0.10848823,0.00007885254,0.000094370356,0.0075678914,0.0005309616,0.685819,0.037914243,0.14668435,0.011632515,0.00016370475],"about_ca_topic_score_codex":0.00057847565,"about_ca_topic_score_gemma":0.00015478935,"teacher_disagreement_score":0.0011639118,"about_ca_system_score_codex":0.00035372257,"about_ca_system_score_gemma":0.00007958341,"threshold_uncertainty_score":0.003019154},"labels":[],"label_agreement":null},{"id":"W2527192255","doi":"10.3847/1538-4357/835/1/21","title":"HARMONIC SPACE ANALYSIS OF PULSAR TIMING ARRAY REDSHIFT MAPS","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Cosmic microwave background; Spectral density; Gravitational wave; Astrophysics; Quadrupole; Gravitational wave background; Gravitational-wave observatory; Redshift; Isotropy; Astronomy; Anisotropy; Optics; Quantum mechanics; Galaxy","score_opus":0.024336009057485397,"score_gpt":0.3384590975900932,"score_spread":0.3141230885326078,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2527192255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.67011094,0.00015831002,0.31700844,0.00018406767,0.00004210461,0.000027019107,0.00054854446,0.00039318137,0.011527541],"genre_scores_gemma":[0.9860811,0.00008835152,0.011819792,0.000017812785,0.00004848509,0.000008386085,0.00031001982,0.00009608914,0.0015299456],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998479,0.000029768844,0.000005185952,0.000027838,0.000067855326,0.00002136731],"domain_scores_gemma":[0.9992217,0.0003617717,0.00015123391,0.00011354518,0.0001112884,0.000040510036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038422397,0.00018351106,0.00013338287,0.0011926447,0.00014365574,0.0005855268,0.00022086565,0.00011067016,0.0030246973],"category_scores_gemma":[0.0026433168,0.0001088857,0.00017075274,0.0005931508,0.00027386655,0.0005144491,0.00034641026,0.0002706662,0.00025980046],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021733031,0.00006667592,0.07464564,0.000092199865,0.00016672106,0.00035671747,0.0003358893,0.4080143,0.04937414,0.26290426,0.0024491115,0.20137715],"study_design_scores_gemma":[0.000011294798,0.000032812248,0.07675372,0.000007399246,0.000018075978,0.0001594315,0.00006816937,0.88020766,0.0060443934,0.03324055,0.0034295898,0.00002694294],"about_ca_topic_score_codex":0.0013721713,"about_ca_topic_score_gemma":0.000832005,"teacher_disagreement_score":0.0030246973,"about_ca_system_score_codex":0.00029192283,"about_ca_system_score_gemma":0.00015236276,"threshold_uncertainty_score":0.010118604},"labels":[],"label_agreement":null},{"id":"W2528137578","doi":"10.3847/1538-4357/833/2/168","title":"THE DRAGONFLY NEARBY GALAXIES SURVEY. II. ULTRA-DIFFUSE GALAXIES NEAR THE ELLIPTICAL GALAXY NGC 5485","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Elliptical galaxy; Galaxy group; Lenticular galaxy; Surface brightness; Brightest cluster galaxy; Peculiar galaxy; Galaxy; Interacting galaxy; Galaxy cluster","score_opus":0.009780848928207641,"score_gpt":0.21540531565853088,"score_spread":0.20562446673032325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2528137578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958702,0.00030476178,0.000121508856,0.000041404946,0.0000039419997,0.0000096053,0.0016489342,0.000029260378,0.0019705163],"genre_scores_gemma":[0.9948048,0.00012213233,0.0003798768,0.00004045794,0.000009223258,0.000006466909,0.003582202,0.0000043554287,0.0010505272],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986994,0.000011290869,0.000005571408,0.00004947477,0.000027258695,0.00003636606],"domain_scores_gemma":[0.99979836,0.000016086984,0.00007054089,0.00002805612,0.0000158361,0.0000711516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015558263,0.00019053719,0.00014659739,0.0019312091,0.00042099057,0.0003747558,0.00021433095,0.00017130199,0.0014071052],"category_scores_gemma":[0.00018546045,0.00010621545,0.00010975573,0.0009442375,0.00019609625,0.0002625543,0.00052390725,0.00012721274,0.00024614367],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000160173,0.00004384339,0.95534384,0.000043812295,0.000071373644,0.00030165366,0.0004547467,0.00018073013,0.009268643,0.00037186843,0.0037241692,0.030035011],"study_design_scores_gemma":[0.0000036622105,0.00001133032,0.997399,0.000004787495,0.000009766407,0.000102712416,0.0000969909,0.00008366921,0.00029390142,0.000015209551,0.0019771892,0.0000017667086],"about_ca_topic_score_codex":0.024625728,"about_ca_topic_score_gemma":0.08979567,"teacher_disagreement_score":0.024625728,"about_ca_system_score_codex":0.00051629194,"about_ca_system_score_gemma":0.000119388926,"threshold_uncertainty_score":0.04896474},"labels":[],"label_agreement":null},{"id":"W2528443618","doi":"10.3847/1538-4357/aaf1a1","title":"How Are Galaxies Assigned to Halos? Searching for Assembly Bias in the SDSS Galaxy Clustering","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Leibniz-Rechenzentrum; Gauss Centre for Supercomputing; Leibniz-Gemeinschaft; York University; Partnership for Advanced Computing in Europe AISBL; National Science Foundation","keywords":"Halo; Galaxy; Galactic halo; Dark matter halo; Dark matter; Galaxy formation and evolution; Sky","score_opus":0.02376554417700667,"score_gpt":0.2505527837873272,"score_spread":0.22678723961032055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2528443618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978835,0.000038207294,0.0014425787,0.000035780708,8.7715796e-7,0.0000030590284,0.00028066913,0.000038582388,0.0002767801],"genre_scores_gemma":[0.9993617,0.000009050552,0.00028599534,0.0000057983384,0.0000010033101,0.0000010137205,0.0002852196,0.000005549343,0.000044652497],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995253,0.00018535054,0.00002569731,0.0001348122,0.0000717955,0.0000569041],"domain_scores_gemma":[0.9957562,0.0017871729,0.00089500175,0.00076327275,0.0004439229,0.0003543166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016331364,0.00021480968,0.00034220127,0.0011360277,0.00030974374,0.0009736983,0.0005710408,0.00032451755,0.0009848038],"category_scores_gemma":[0.0066402573,0.00018823448,0.00043772333,0.0011444935,0.00043252445,0.00050098944,0.0005210628,0.0002067057,0.00015846462],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016342528,0.00001953332,0.9555724,0.000018493669,0.00012137834,0.000037992533,0.0001326105,0.037243776,0.0017691378,0.0013967991,0.00027809438,0.00324633],"study_design_scores_gemma":[0.00001678648,0.000057892958,0.69097185,0.000015433403,0.0000712601,0.000054582848,0.00022966786,0.30338374,0.0021595247,0.0025791118,0.00043968085,0.000020428359],"about_ca_topic_score_codex":0.018763857,"about_ca_topic_score_gemma":0.013138584,"teacher_disagreement_score":0.018763857,"about_ca_system_score_codex":0.00082907476,"about_ca_system_score_gemma":0.00032647065,"threshold_uncertainty_score":0.03730929},"labels":[],"label_agreement":null},{"id":"W2528505744","doi":"10.3847/1538-4357/833/1/97","title":"INFALL/EXPANSION VELOCITIES IN THE LOW-MASS DENSE CORES L492, L694-2, AND L1521F: DEPENDENCE ON POSITION AND MOLECULAR TRACER","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Core (optical fiber); Telescope; Position (finance); Line (geometry); Offset (computer science); James Clerk Maxwell Telescope; Radial velocity","score_opus":0.006117380630065991,"score_gpt":0.22166266901202844,"score_spread":0.21554528838196246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2528505744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996544,0.000019817302,0.00004206087,0.0000035582955,3.536092e-7,0.0000010928107,0.00007948972,0.000005728934,0.00019348811],"genre_scores_gemma":[0.99973136,0.0000059395215,0.000051747484,0.0000029383282,7.968218e-7,0.0000012969303,0.0001561124,0.0000017514413,0.00004800625],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999176,0.0000056738118,0.0000044731464,0.000024227744,0.000016227885,0.00003178193],"domain_scores_gemma":[0.99952614,0.00006681024,0.00016828864,0.000020848414,0.00007725284,0.00014072606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021157003,0.00017690632,0.00019382873,0.0008699814,0.00029950097,0.00040353002,0.00033624942,0.0002505016,0.0008183616],"category_scores_gemma":[0.0005375625,0.000114142844,0.00017514468,0.00030747944,0.00022524489,0.00032871333,0.00043309404,0.00016857155,0.00020528349],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021798025,0.00005388448,0.967362,0.000009731259,0.000027424321,0.00011938684,0.0001396426,0.0005222934,0.028876213,0.000047352903,0.00009954256,0.0025245985],"study_design_scores_gemma":[0.000003353202,0.000019456813,0.99804854,0.0000013453449,0.0000029846813,0.000032583222,0.000058509406,0.00091382343,0.0008561039,0.00000773616,0.000053588738,0.0000019607273],"about_ca_topic_score_codex":0.015841227,"about_ca_topic_score_gemma":0.024428073,"teacher_disagreement_score":0.015841227,"about_ca_system_score_codex":0.00052662013,"about_ca_system_score_gemma":0.000109431545,"threshold_uncertainty_score":0.031498015},"labels":[],"label_agreement":null},{"id":"W2528756926","doi":"10.3847/0004-637x/832/2/148","title":"MOLECULAR GAS ALONG A BRIGHT Hα FILAMENT IN 2A 0335+096 REVEALED BY ALMA","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Manitoba; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Canadian Space Agency; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; National Science Council; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Protein filament; Galaxy; Molecular cloud; Intracluster medium; Redshift; Cluster (spacecraft); RADIUS; Outflow","score_opus":0.0040959224818439745,"score_gpt":0.19677682826445436,"score_spread":0.19268090578261038,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2528756926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99949765,0.0000415482,0.000048905018,0.00001475111,0.000001728458,0.0000021070296,0.000052160947,0.00000997504,0.000331076],"genre_scores_gemma":[0.99977857,0.0000073255255,0.00007579389,0.0000096835,0.0000045558895,0.0000010788748,0.00006741255,0.0000012864897,0.0000542196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999361,0.000004771669,0.000003061333,0.000019867151,0.000014840992,0.000021210744],"domain_scores_gemma":[0.99986434,0.000008811438,0.000043218522,0.000011340403,0.000016555516,0.00005569701],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009055293,0.00014732861,0.00019013719,0.0007587033,0.00046916833,0.0004311627,0.00027723922,0.00030598626,0.00081219635],"category_scores_gemma":[0.00017785399,0.00012531481,0.00016730763,0.00041457292,0.00023493683,0.00016643092,0.00028703053,0.00016031864,0.00015736047],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038948847,0.00010237858,0.8574193,0.000024041925,0.0000774279,0.0025662691,0.0006696974,0.00038686127,0.13210571,0.00021767462,0.00042785206,0.005613309],"study_design_scores_gemma":[0.000006150936,0.000049355323,0.99743783,0.0000023268767,0.000015194486,0.0004065201,0.00010382933,0.0006050201,0.0008674095,0.000039054667,0.0004639956,0.0000032795513],"about_ca_topic_score_codex":0.006903034,"about_ca_topic_score_gemma":0.010352048,"teacher_disagreement_score":0.006903034,"about_ca_system_score_codex":0.0003509739,"about_ca_system_score_gemma":0.00007880495,"threshold_uncertainty_score":0.013725698},"labels":[],"label_agreement":null},{"id":"W2529217009","doi":"10.3847/1538-4357/833/2/167","title":"THE PAndAS VIEW OF THE ANDROMEDA SATELLITE SYSTEM. II. DETAILED PROPERTIES OF 23 M31 DWARF SPHEROIDAL GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":155,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Dwarf spheroidal galaxy; Dwarf galaxy; Dwarf galaxy problem; Andromeda; Galaxy; Luminosity; Satellite galaxy; Elliptical galaxy","score_opus":0.009142229528702724,"score_gpt":0.1927077746468679,"score_spread":0.18356554511816517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2529217009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7275391,0.0061434014,0.009759336,0.0009801672,0.0001107749,0.00009642122,0.14842933,0.005093659,0.10184786],"genre_scores_gemma":[0.92007643,0.0012933897,0.016370239,0.00014612028,0.00010920009,0.000035578072,0.0533073,0.00051958265,0.008142163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983656,0.000023088243,0.0000063173525,0.000057116384,0.00005166949,0.000025132418],"domain_scores_gemma":[0.99971896,0.000038119284,0.000069989044,0.00007573757,0.0000520775,0.00004514034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000206768,0.0003442644,0.00018928666,0.002272494,0.00042349903,0.00084478484,0.0002851303,0.00019626178,0.0060273143],"category_scores_gemma":[0.0003985262,0.00021644146,0.0002638723,0.0015730574,0.00016996555,0.0005357106,0.000602142,0.0002807699,0.0022774346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054762105,0.00011059373,0.61532456,0.00063831464,0.00039073717,0.0005235587,0.0012156748,0.010023676,0.028183129,0.013124837,0.07976362,0.2501537],"study_design_scores_gemma":[0.000011254552,0.00004738827,0.8123164,0.00006890817,0.00006888662,0.0006828829,0.00036329255,0.0043985494,0.0026706909,0.0020796238,0.17725581,0.00003625493],"about_ca_topic_score_codex":0.017155807,"about_ca_topic_score_gemma":0.035113182,"teacher_disagreement_score":0.017155807,"about_ca_system_score_codex":0.000334749,"about_ca_system_score_gemma":0.00030039088,"threshold_uncertainty_score":0.034111857},"labels":[],"label_agreement":null},{"id":"W2529381469","doi":"10.3847/1538-4357/834/1/35","title":"THE NANOGRAV NINE-YEAR DATA SET: EXCESS NOISE IN MILLISECOND PULSAR ARRIVAL TIMES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; California Institute of Technology; National Aeronautics and Space Administration; Universities Space Research Association; National Radio Astronomy Observatory; National Science Foundation","keywords":"Millisecond pulsar; Noise (video); Pulsar; Achromatic lens; Observatory; Scaling; Gravitational wave; Chromatic scale; Noise power","score_opus":0.021586024735718454,"score_gpt":0.32554089148183496,"score_spread":0.3039548667461165,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2529381469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9892077,0.00016995324,0.0023853206,0.00018735946,0.000035976067,0.000010852726,0.0066393474,0.00009857184,0.001264937],"genre_scores_gemma":[0.9813743,0.000056171102,0.0011035218,0.000059647453,0.000031446212,0.000012265265,0.017073808,0.000030530817,0.00025832103],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993325,0.000114325805,0.00007814595,0.0001995445,0.00021832837,0.000057135574],"domain_scores_gemma":[0.9962662,0.001326132,0.0007663266,0.0009283099,0.0004967961,0.00021619191],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013392083,0.00020383354,0.0003998711,0.0017670493,0.0003889891,0.0007836127,0.0005627255,0.0004040102,0.00079010014],"category_scores_gemma":[0.004287477,0.00010969943,0.00026632805,0.0021762114,0.00034847815,0.00056015124,0.00074254966,0.00045110978,0.00034727843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005250086,0.00016062649,0.9404363,0.000102581376,0.00023829717,0.00046994298,0.0002455539,0.013085091,0.007928618,0.0015838593,0.0062459,0.028978297],"study_design_scores_gemma":[0.000033252494,0.000061794126,0.9653125,0.00002183528,0.000042858435,0.000369302,0.00016505265,0.023757452,0.0026673863,0.000719326,0.006822774,0.00002660296],"about_ca_topic_score_codex":0.005414611,"about_ca_topic_score_gemma":0.0067369635,"teacher_disagreement_score":0.005414611,"about_ca_system_score_codex":0.00030950407,"about_ca_system_score_gemma":0.00022805264,"threshold_uncertainty_score":0.010766149},"labels":[],"label_agreement":null},{"id":"W2529413960","doi":"10.3847/1538-4357/833/1/103","title":"KILOPARSEC-SCALE DUST DISKS IN HIGH-REDSHIFT LUMINOUS SUBMILLIMETER GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":312,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Dalhousie University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Deutsche Forschungsgemeinschaft; Aspen Center for Physics; National Radio Astronomy Observatory; Vetenskapsrådet; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Astronomy; Luminous infrared galaxy; Cosmic dust","score_opus":0.00789918772406073,"score_gpt":0.20341404755717424,"score_spread":0.1955148598331135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2529413960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942493,0.0000692346,0.00012927671,0.000010911026,0.0000010932415,0.0000015690488,0.00008098514,0.000018724055,0.00026330783],"genre_scores_gemma":[0.99968004,0.000018549586,0.0001532485,0.000006367925,0.000003244886,0.0000011550716,0.00009572146,0.0000018490973,0.000039968265],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999317,0.00000928702,0.000004629381,0.000020793499,0.000014638051,0.000018877561],"domain_scores_gemma":[0.9994542,0.00013509412,0.0002080208,0.00006742025,0.000035369016,0.00009991948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002312984,0.00016854182,0.00015558989,0.0008646049,0.00018649692,0.00059542776,0.00031991006,0.00022279628,0.0009193649],"category_scores_gemma":[0.0006579546,0.000160001,0.00022565352,0.00040897934,0.0002636789,0.0002506602,0.00035395482,0.00016518983,0.00017314266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013611774,0.00004945803,0.96738607,0.00003142197,0.00008138588,0.00019327109,0.00020681875,0.002314049,0.024066124,0.00021055143,0.00017207551,0.0051527754],"study_design_scores_gemma":[0.0000047171225,0.00002133178,0.99757046,0.0000027968824,0.0000106325215,0.00006278943,0.0000491445,0.0014797703,0.0005864539,0.00007913836,0.00013065927,0.0000019971953],"about_ca_topic_score_codex":0.0029836814,"about_ca_topic_score_gemma":0.003260758,"teacher_disagreement_score":0.0029836814,"about_ca_system_score_codex":0.0003227902,"about_ca_system_score_gemma":0.00007505607,"threshold_uncertainty_score":0.005932629},"labels":[],"label_agreement":null},{"id":"W2529707025","doi":"10.3847/1538-4357/836/1/54","title":"Testing the Large-scale Environments of Cool-core and Non-cool-core Clusters with Clustering Bias","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Cluster (spacecraft); Redshift; Galaxy cluster; Cluster analysis; Kullback–Leibler divergence; Entropy (arrow of time); Galaxy","score_opus":0.021535033248679503,"score_gpt":0.22505072680239976,"score_spread":0.20351569355372026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2529707025","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993536,0.000018052919,0.0004083771,0.0000057640864,9.987389e-7,0.0000016413472,0.000037847418,0.000007963387,0.00016572462],"genre_scores_gemma":[0.99972135,0.0000031533837,0.00017378655,0.0000031482696,0.0000011182931,0.0000010345757,0.00006574351,0.0000029147573,0.000027750111],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999316,0.00016822887,0.000034516794,0.0002394387,0.00014035488,0.00010145688],"domain_scores_gemma":[0.99487996,0.0019405866,0.0010445149,0.0007433876,0.0007038625,0.0006877166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020245374,0.00019189712,0.00026363565,0.0010695736,0.00052752515,0.0007883857,0.00035758442,0.00027805907,0.0010396666],"category_scores_gemma":[0.005263598,0.00013474932,0.00021523121,0.00059716176,0.00082072517,0.00038917977,0.0010206136,0.0002258384,0.00016715105],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013190335,0.000014610223,0.98975706,0.000008606166,0.00005679209,0.000018630175,0.0001306053,0.00078279973,0.006461265,0.0002085658,0.00006001473,0.0023690516],"study_design_scores_gemma":[0.0000048093034,0.000029568164,0.99244106,0.0000025094735,0.000019661135,0.000028455255,0.00011686118,0.0047886777,0.0023158242,0.00015140395,0.00009505587,0.0000061602987],"about_ca_topic_score_codex":0.007349426,"about_ca_topic_score_gemma":0.006877313,"teacher_disagreement_score":0.007349426,"about_ca_system_score_codex":0.0005339218,"about_ca_system_score_gemma":0.0002373468,"threshold_uncertainty_score":0.01461333},"labels":[],"label_agreement":null},{"id":"W2529773886","doi":"10.3847/0004-637x/833/1/6","title":"A SYSTEMATIC SEARCH FOR PERIODICALLY VARYING QUASARS IN PAN-STARRS1: AN EXTENDED BASELINE TEST IN MEDIUM DEEP SURVEY FIELD MD09","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Office of Science; Max-Planck-Institut für Astronomie; National Central University; Lawrence Berkeley National Laboratory; Ministerio de Ciencia, Tecnología e Innovación Productiva; Durham University; York University; Space Telescope Science Institute; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Brookhaven National Laboratory; Ministério da Ciência, Tecnologia e Inovação; Northern Arizona University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Science Mission Directorate; Yale University; Vanderbilt University; National Science Foundation; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; U.S. Department of Energy","keywords":"Quasar; Supermassive black hole; Light curve; Binary number; Sample (material); Channel (broadcasting); Baseline (sea)","score_opus":0.01508719578252098,"score_gpt":0.2549859531774575,"score_spread":0.2398987573949365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2529773886","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992119,0.000022044169,0.00020882956,0.000012294059,0.0000010057192,0.0000044776093,0.00038182814,0.0000096622225,0.00014788377],"genre_scores_gemma":[0.9979182,0.000012611852,0.0005124609,0.00001523395,0.0000036280346,0.000008546458,0.0014163451,0.0000042875713,0.000108684835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994647,0.00012285488,0.000035263023,0.0001831287,0.00010960526,0.0000844106],"domain_scores_gemma":[0.99743795,0.0005376144,0.0007642134,0.00048896275,0.00031588296,0.00045534023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010844014,0.00016285967,0.00023230401,0.0015279286,0.00041601775,0.00040803207,0.00049644086,0.00019279304,0.0008643405],"category_scores_gemma":[0.001993699,0.00014571451,0.0002327241,0.00061101496,0.00032056007,0.00028761703,0.0008381962,0.00018366825,0.000217265],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011113488,0.00003522802,0.9862368,0.000013989357,0.000045511984,0.00008313273,0.0001029956,0.00015318561,0.0090635605,0.00007051596,0.00022267002,0.003861304],"study_design_scores_gemma":[0.0000058969085,0.000060099268,0.9980356,0.0000020512973,0.000014500951,0.000104483246,0.00009354463,0.00062740373,0.0006920522,0.000016678687,0.00034496398,0.000002885315],"about_ca_topic_score_codex":0.0046453658,"about_ca_topic_score_gemma":0.01293591,"teacher_disagreement_score":0.0046453658,"about_ca_system_score_codex":0.00029113598,"about_ca_system_score_gemma":0.00026962694,"threshold_uncertainty_score":0.009236693},"labels":[],"label_agreement":null},{"id":"W2529873760","doi":"10.3847/1538-4357/833/1/83","title":"EVOLUTION OF CATACLYSMIC VARIABLES AND RELATED BINARIES CONTAINING A WHITE DWARF","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Bishop's University","funders":"","keywords":"White dwarf; Orbital period; Accretion (finance); Cataclysmic variable star; Binary number; Population; Binary star; Orbital plane","score_opus":0.00797922289837154,"score_gpt":0.20816000463792908,"score_spread":0.20018078173955753,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2529873760","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99910873,0.000039954793,0.00027680167,0.000009195203,0.0000013812096,0.0000024254348,0.00008651711,0.0000062747777,0.00046870927],"genre_scores_gemma":[0.9994155,0.000009847239,0.00022361997,0.0000025881334,0.0000011785775,0.0000019024606,0.00021779767,0.0000031535076,0.00012437416],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99982977,0.00004598038,0.0000126061595,0.000054787182,0.000025939777,0.000030792966],"domain_scores_gemma":[0.9992254,0.000329108,0.00016576784,0.00007067224,0.00007856746,0.00013038582],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004222683,0.00015803578,0.00022609114,0.0010191858,0.0005711926,0.0011166943,0.0003262569,0.00025594272,0.0012523476],"category_scores_gemma":[0.0016316865,0.00011191018,0.0002320428,0.0007917152,0.00035226697,0.00047456083,0.0007197779,0.00026204964,0.00014589804],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001803292,0.00006663291,0.9679567,0.000015405281,0.000054439766,0.00019747516,0.00015023634,0.021194806,0.0020511574,0.0022055733,0.00019370294,0.005733466],"study_design_scores_gemma":[0.000031898006,0.00015402415,0.8166257,0.000016998063,0.000040184546,0.0005021347,0.0005495948,0.17431034,0.0025775821,0.0035893973,0.0015820444,0.000020098701],"about_ca_topic_score_codex":0.006691951,"about_ca_topic_score_gemma":0.006432444,"teacher_disagreement_score":0.006691951,"about_ca_system_score_codex":0.0006204578,"about_ca_system_score_gemma":0.00020247143,"threshold_uncertainty_score":0.013306022},"labels":[],"label_agreement":null},{"id":"W2530399778","doi":"10.3847/1538-4357/833/2/202","title":"THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT. II. ISOLATED DISK TEST","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":140,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Galaxy; Supernova; Milky Way; Galaxy formation and evolution; Star formation; Radiative transfer; Computational astrophysics; Radiative cooling; Thin disk","score_opus":0.010536020658782043,"score_gpt":0.23869624280837626,"score_spread":0.22816022214959422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2530399778","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8670878,0.0010164789,0.022337744,0.0014054967,0.0007508929,0.00051529176,0.043468587,0.020302866,0.043114807],"genre_scores_gemma":[0.8899162,0.00021045125,0.055581655,0.0006622575,0.000112211026,0.00049778144,0.045187417,0.0045507373,0.0032813197],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991279,0.00028867793,0.000053247088,0.00016665927,0.00023726058,0.0001262793],"domain_scores_gemma":[0.9976962,0.0009216485,0.00014727649,0.0005073052,0.00047045352,0.0002570682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018844457,0.00087854126,0.00064066617,0.00078689994,0.00052285765,0.0008847644,0.002709143,0.0014252275,0.004430159],"category_scores_gemma":[0.0049035577,0.0003756362,0.0009828816,0.0008520526,0.000526238,0.0011441965,0.001200209,0.0016191178,0.0013944648],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031874499,0.0024038805,0.0723833,0.00131303,0.0012470989,0.00088735507,0.0006215323,0.66915035,0.014003674,0.025045242,0.15371166,0.05604542],"study_design_scores_gemma":[0.0011513878,0.0005739405,0.015428747,0.0000631147,0.00009169343,0.00015505403,0.00020695818,0.93639547,0.008390984,0.0051305266,0.03233906,0.00007304919],"about_ca_topic_score_codex":0.011491097,"about_ca_topic_score_gemma":0.011503078,"teacher_disagreement_score":0.011491097,"about_ca_system_score_codex":0.0006778774,"about_ca_system_score_gemma":0.000746439,"threshold_uncertainty_score":0.022848427},"labels":[],"label_agreement":null},{"id":"W2530650773","doi":"10.3847/0004-637x/832/2/184","title":"PROTOSTELLAR OUTFLOWS IN L1340","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"University of California, Los Angeles; Centre National de la Recherche Scientifique; Liverpool John Moores University; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory","keywords":"Protostar; Outflow; Stars; Population; Shock (circulatory); Molecular cloud; Line (geometry)","score_opus":0.009855764864434612,"score_gpt":0.2344723773197503,"score_spread":0.22461661245531567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2530650773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997285,0.000015191854,0.00003534702,0.0000054341403,4.691297e-7,0.0000015234399,0.000055054083,0.0000062918575,0.00015208243],"genre_scores_gemma":[0.9995778,0.000009100056,0.00011010423,0.000010944723,9.984038e-7,0.0000011082574,0.00014979244,0.000001728946,0.00013851792],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999294,0.0000055038026,0.000003800669,0.000013055006,0.000015220911,0.00003287902],"domain_scores_gemma":[0.9997888,0.000016207623,0.00007709311,0.000007083308,0.00002321409,0.00008757983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009635181,0.00014020911,0.000114265466,0.00055762276,0.0003783204,0.0002727612,0.00015386872,0.00014607552,0.0011070005],"category_scores_gemma":[0.00025337972,0.00008159741,0.00011197647,0.00042583386,0.00018557328,0.00011694142,0.00042176244,0.00015826499,0.00015869552],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003040986,0.00007966928,0.9222447,0.00002483402,0.000024079305,0.0004480705,0.00028945043,0.00027683476,0.06828191,0.00016026828,0.0001869608,0.0076789907],"study_design_scores_gemma":[0.000005393313,0.000089631234,0.9966235,0.000002820508,0.000005581757,0.00026483665,0.00011346529,0.00025943524,0.0021389555,0.000044629083,0.00044802757,0.0000037252084],"about_ca_topic_score_codex":0.0074266396,"about_ca_topic_score_gemma":0.010445682,"teacher_disagreement_score":0.0074266396,"about_ca_system_score_codex":0.0003844368,"about_ca_system_score_gemma":0.00016975372,"threshold_uncertainty_score":0.014766872},"labels":[],"label_agreement":null},{"id":"W2530773550","doi":"10.3847/0004-637x/832/2/183","title":"TATOOINE’S FUTURE: THE ECCENTRIC RESPONSE OF KEPLER’S CIRCUMBINARY PLANETS TO COMMON-ENVELOPE EVOLUTION OF THEIR HOST STARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto; York University","funders":"","keywords":"Circumbinary planet; Kepler-47; Planet; Binary star; Planetary system; Orbit (dynamics); Binary number; Orbital elements","score_opus":0.008962779757955132,"score_gpt":0.21458187113631433,"score_spread":0.2056190913783592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2530773550","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99803275,0.000055244942,0.00040951578,0.00006559179,0.000003377289,0.0000013394539,0.000036984406,0.000010046028,0.0013852122],"genre_scores_gemma":[0.9996861,0.00001656684,0.00010843543,0.000006889805,9.502713e-7,8.561153e-7,0.000029162853,0.000004220688,0.00014687929],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999553,0.000010260017,0.0000013823126,0.000015648895,0.0000061888422,0.0000111739855],"domain_scores_gemma":[0.9997075,0.00011594729,0.000053887026,0.000029690304,0.000025203142,0.000067749],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023997886,0.00016249125,0.00018279749,0.00023582038,0.0003764304,0.0007231764,0.00029806016,0.00040271858,0.0015632398],"category_scores_gemma":[0.0012979048,0.00013762602,0.0002518621,0.00018078125,0.00032056007,0.000730249,0.00047046528,0.00038419556,0.0001578552],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007512852,0.000241697,0.3787284,0.00007653877,0.00029726332,0.0007073799,0.00067665975,0.55921024,0.029685361,0.01557733,0.0015224395,0.012525385],"study_design_scores_gemma":[0.000050596496,0.00018520972,0.14001043,0.000015850766,0.000046324913,0.00015766677,0.0004101583,0.849464,0.0028929599,0.0049050963,0.0018278601,0.000033862594],"about_ca_topic_score_codex":0.0056491466,"about_ca_topic_score_gemma":0.0041571674,"teacher_disagreement_score":0.0056491466,"about_ca_system_score_codex":0.00056691,"about_ca_system_score_gemma":0.00020149424,"threshold_uncertainty_score":0.011232555},"labels":[],"label_agreement":null},{"id":"W2531052858","doi":"10.3847/1538-4357/aa6d0c","title":"A Near-infrared Counterpart of 2E1613.5–5053: The Central Source in Supernova Remnant RCW103","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; University of Leicester; Space Telescope Science Institute; National Aeronautics and Space Administration; Canada Research Chairs; McGill University","keywords":"Supernova remnant; Neutron star; Near-Earth supernova; H II region; Binary number; Infrared; Hubble space telescope; Binary star","score_opus":0.012024756978740767,"score_gpt":0.23915197928395865,"score_spread":0.22712722230521787,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2531052858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957296,0.00013684883,0.0002544734,0.00008268801,0.000024082454,0.000016624668,0.00031612304,0.000040212,0.0033993316],"genre_scores_gemma":[0.9978728,0.000048982685,0.00043819513,0.00007013636,0.000021444592,0.000008152865,0.0006249225,0.000013227679,0.0009021629],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998894,0.000005256676,0.0000075390813,0.000034558805,0.000030248466,0.00003298508],"domain_scores_gemma":[0.9995098,0.000028454091,0.00016135274,0.00006758552,0.000025641637,0.00020717471],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015574085,0.0003338321,0.00044053653,0.00056047086,0.00086719316,0.00060150016,0.00041994566,0.0007910591,0.002505294],"category_scores_gemma":[0.000292848,0.00022895352,0.0003136054,0.0006157761,0.0005120458,0.00022507466,0.00074004673,0.0006627527,0.0009136699],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001235033,0.0005819277,0.5847068,0.00017004523,0.00016221417,0.042348154,0.0017505288,0.00048543187,0.33298132,0.0018047328,0.004025331,0.029748533],"study_design_scores_gemma":[0.000044205433,0.0002824539,0.97312886,0.00003075665,0.000028322629,0.012619358,0.00038428276,0.00042887955,0.008505473,0.00025911373,0.004268481,0.00001988046],"about_ca_topic_score_codex":0.0033312568,"about_ca_topic_score_gemma":0.0077324426,"teacher_disagreement_score":0.0033312568,"about_ca_system_score_codex":0.00042457387,"about_ca_system_score_gemma":0.00020318873,"threshold_uncertainty_score":0.008381069},"labels":[],"label_agreement":null},{"id":"W2531108515","doi":"10.3847/1538-4357/833/1/118","title":"THE LINEAR INSTABILITY OF DILUTE ULTRARELATIVISTIC e<sup>±</sup> PAIR BEAMS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Kinetic energy; Instability; Plasma; Beam (structure); Atomic physics; Lorentz factor; Anisotropy; Computational physics; Lorentz transformation; Nuclear physics; Optics; Classical mechanics; Mechanics","score_opus":0.008359342056778839,"score_gpt":0.21559444763091298,"score_spread":0.20723510557413413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2531108515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96681166,0.00021447666,0.022367528,0.00013308816,0.000021549347,0.000026626341,0.000058337755,0.00010886275,0.010257869],"genre_scores_gemma":[0.9972263,0.0000630278,0.0012143644,0.000033576503,0.0000059293975,0.000015668345,0.00003620328,0.000012073659,0.0013927565],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998852,0.000026277407,0.000005085642,0.000016086082,0.00003652364,0.000030826468],"domain_scores_gemma":[0.999637,0.00012730881,0.00011777252,0.000024451312,0.000050347655,0.00004302904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031604557,0.00033279712,0.00021271489,0.00029064092,0.00034704924,0.0007366587,0.00053493143,0.00042165912,0.0020611421],"category_scores_gemma":[0.000965628,0.00025493567,0.00026924393,0.00027630644,0.00068542344,0.00054841465,0.0006583021,0.00035026792,0.00030394492],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005995402,0.00019323699,0.050645243,0.0002432313,0.00025838875,0.0013832322,0.0008439674,0.44119787,0.31423363,0.16834317,0.00228869,0.019769805],"study_design_scores_gemma":[0.00009046985,0.00012935774,0.019796215,0.000015330254,0.000033310134,0.00028068555,0.00020899539,0.9158835,0.048596967,0.013539815,0.0013773427,0.000048057984],"about_ca_topic_score_codex":0.0014003742,"about_ca_topic_score_gemma":0.0008000321,"teacher_disagreement_score":0.0020611421,"about_ca_system_score_codex":0.00042955272,"about_ca_system_score_gemma":0.00020258459,"threshold_uncertainty_score":0.0068951845},"labels":[],"label_agreement":null},{"id":"W2531334071","doi":"10.3847/1538-4357/aa69c2","title":"The RAVE-on Catalog of Stellar Atmospheric Parameters and Chemical Abundances for Chemo-dynamic Studies in the Gaia Era","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leibniz-Gemeinschaft; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Max-Planck-Institut für Astronomie; Istituto Nazionale di Astrofisica; Javna Agencija za Raziskovalno Dejavnost RS; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Australian Astronomical Optics-Macquarie; Deutsche Forschungsgemeinschaft; Macquarie University; Australian Research Council; Vanderbilt University; King's College London; European Commission; Johns Hopkins University; Simons Foundation; Agence Nationale de la Recherche; W. M. Keck Foundation; Australian National University; National Aeronautics and Space Administration; University of Cambridge; National Science Foundation","keywords":"Milky Way; Stars; Physics; Astrophysics; Surface gravity; Galaxy; Spectral line; Astronomy; Giant star; Galaxy formation and evolution","score_opus":0.02152068453413826,"score_gpt":0.28175087997380205,"score_spread":0.2602301954396638,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2531334071","genre_codex":"empirical","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58871824,0.001614015,0.041431356,0.0003278471,0.00008963996,0.00039493298,0.31223404,0.0182226,0.03696739],"genre_scores_gemma":[0.48853165,0.00053698977,0.06922129,0.00026008376,0.00009465447,0.00031876436,0.43157935,0.0019938084,0.007463407],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.999424,0.00006293593,0.000046772053,0.00018880893,0.000215427,0.00006207517],"domain_scores_gemma":[0.9969463,0.00019691681,0.00050591165,0.0014751616,0.0006612329,0.00021447893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015405355,0.00051510683,0.0005229456,0.0038082208,0.00028969618,0.00096587784,0.0008516321,0.0003899487,0.003217538],"category_scores_gemma":[0.0030825883,0.0003244176,0.0006624338,0.0027853756,0.00019725329,0.0008830063,0.0015565397,0.00036302983,0.003076857],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054946635,0.0001874142,0.63715124,0.00066239276,0.0006397653,0.00030524566,0.0006154952,0.019292802,0.02580634,0.009282238,0.09240881,0.21309896],"study_design_scores_gemma":[0.0001114101,0.00013506129,0.64745307,0.00015364114,0.00019485882,0.00022632492,0.00014353415,0.018325943,0.009552423,0.0032024572,0.32044265,0.00005861177],"about_ca_topic_score_codex":0.010579499,"about_ca_topic_score_gemma":0.013390795,"teacher_disagreement_score":0.010579499,"about_ca_system_score_codex":0.00050570426,"about_ca_system_score_gemma":0.001010169,"threshold_uncertainty_score":0.02103585},"labels":[],"label_agreement":null},{"id":"W2531492754","doi":"10.3847/1538-4357/aa5c8d","title":"Advanced LIGO Constraints on Neutron Star Mergers and r-process Sites","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"LIGO; Physics; Neutron star; Astrophysics; Gravitational wave; r-process; Population; Context (archaeology); Nucleosynthesis; Metallicity; Stars","score_opus":0.012743163441076689,"score_gpt":0.26155845117143467,"score_spread":0.248815287730358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2531492754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897704,0.0013391884,0.003588086,0.0001762865,0.0000071041427,0.0000050802064,0.00034359618,0.00006767713,0.0047026617],"genre_scores_gemma":[0.9987319,0.00021885236,0.00062597246,0.00002659674,0.000012831792,0.000002713082,0.00024303078,0.000012758407,0.0001252413],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999519,0.0001358104,0.000032366333,0.0001430841,0.00010188078,0.00006780164],"domain_scores_gemma":[0.9975434,0.0012086498,0.0006351304,0.00026855565,0.00013558839,0.00020862186],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019190117,0.0003574646,0.0003761589,0.0012240334,0.00036264453,0.0012555126,0.00041871084,0.00074947753,0.0012890545],"category_scores_gemma":[0.0046358067,0.0003097399,0.0005428036,0.0006788271,0.00078447413,0.0014411398,0.0013267025,0.00039085976,0.00032425742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001057763,0.000083289204,0.7719658,0.00030497406,0.0003358521,0.0008286506,0.00048363672,0.10095032,0.04390475,0.045624632,0.0007190911,0.03374129],"study_design_scores_gemma":[0.00013151277,0.00016404362,0.757689,0.000104437284,0.0002067805,0.0005927407,0.00022983446,0.18911885,0.016362354,0.02565287,0.0096721435,0.00007542859],"about_ca_topic_score_codex":0.002472207,"about_ca_topic_score_gemma":0.0015580032,"teacher_disagreement_score":0.002472207,"about_ca_system_score_codex":0.0009984028,"about_ca_system_score_gemma":0.00024153866,"threshold_uncertainty_score":0.010148823},"labels":[],"label_agreement":null},{"id":"W2531519367","doi":"10.3847/0004-637x/833/1/23","title":"THE SCALING RELATIONS AND STAR FORMATION LAWS OF MINI-STARBURST COMPLEXES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Star formation; Molecular cloud; Milky Way; Scaling; Diagram; Scaling law; Star (game theory); Gravitational collapse","score_opus":0.013817386487371101,"score_gpt":0.2395124072188442,"score_spread":0.2256950207314731,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2531519367","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99541485,0.00020420493,0.0023814782,0.000052777516,0.0000028436855,0.00000963526,0.000077392964,0.000021033326,0.0018357221],"genre_scores_gemma":[0.9994898,0.000034178825,0.00034404232,0.0000048910347,0.0000037173736,0.0000033266278,0.000045007753,0.0000027601554,0.000072294635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998142,0.00003161803,0.000015393418,0.00006269775,0.00004539214,0.000030673753],"domain_scores_gemma":[0.9975916,0.00082578906,0.00084288215,0.00017469612,0.00023201287,0.00033293918],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004927661,0.00014376853,0.0002136943,0.0013076128,0.00026243617,0.0007757916,0.00034082326,0.0001954977,0.001281267],"category_scores_gemma":[0.004471576,0.00011033728,0.00023445346,0.0004764021,0.00061515317,0.0007105962,0.00031537315,0.00022678288,0.00014026756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015022368,0.000060693365,0.8895913,0.00011036437,0.00009505804,0.00062831957,0.0019074291,0.015841935,0.025665993,0.040355243,0.00085219723,0.02474125],"study_design_scores_gemma":[0.000015728157,0.00008095609,0.8841857,0.000029829267,0.00002327763,0.00084240566,0.00052143843,0.083272204,0.0023415885,0.02661202,0.0020449632,0.000029908284],"about_ca_topic_score_codex":0.0022864726,"about_ca_topic_score_gemma":0.0010172186,"teacher_disagreement_score":0.0022864726,"about_ca_system_score_codex":0.0004216663,"about_ca_system_score_gemma":0.00011275941,"threshold_uncertainty_score":0.0045463443},"labels":[],"label_agreement":null},{"id":"W2531959249","doi":"10.3847/1538-4357/834/2/136","title":"TOWARD HIGH-PRECISION SEISMIC STUDIES OF WHITE DWARF STARS: PARAMETRIZATION OF THE CORE AND TESTS OF ACCURACY","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Parametrization (atmospheric modeling); Chemical evolution; Core (optical fiber); Stratification (seeds); Tracing","score_opus":0.041588168016011784,"score_gpt":0.29533498973613975,"score_spread":0.25374682172012797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2531959249","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5164918,0.0002134658,0.4777991,0.00027959514,0.00002617617,0.000047462745,0.00021489395,0.000388637,0.0045389193],"genre_scores_gemma":[0.949463,0.000108987224,0.04946353,0.000026072381,0.00001098823,0.00003731727,0.00013744691,0.00006127714,0.000691438],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985814,0.000055855715,0.000009948563,0.000028206054,0.000033043583,0.000014827429],"domain_scores_gemma":[0.9991598,0.0003505561,0.00014462916,0.00022047362,0.000080157726,0.00004446625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00083106046,0.00057329604,0.00037386405,0.00032393518,0.0002677571,0.00095722463,0.0006294897,0.00086080347,0.00047393295],"category_scores_gemma":[0.0053777713,0.00033211062,0.00031553284,0.000253989,0.00064179156,0.00089516223,0.0009409474,0.0009011556,0.0001400986],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057744735,0.000040984807,0.006274193,0.00003237419,0.00001653457,0.000042816017,0.00008412969,0.9683585,0.0074125137,0.008201133,0.000083798186,0.009395233],"study_design_scores_gemma":[0.000007423118,0.000029022023,0.0009229635,0.0000072870575,0.000003277985,0.000009891333,0.000020407513,0.99477696,0.0016959981,0.0021478275,0.00037294824,0.00000603421],"about_ca_topic_score_codex":0.0046771453,"about_ca_topic_score_gemma":0.002960248,"teacher_disagreement_score":0.0046771453,"about_ca_system_score_codex":0.00036163762,"about_ca_system_score_gemma":0.0004998342,"threshold_uncertainty_score":0.009299874},"labels":[],"label_agreement":null},{"id":"W2532278570","doi":"10.3847/1538-4357/833/2/140","title":"ASSESSING MAGNETIC TORQUES AND ENERGY FLUXES IN CLOSE-IN STAR–PLANET SYSTEMS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planet; Physics; Magnetic energy; Star (game theory); Astrophysics; Kepler-69c; Magnetic field; Planetary system; Magnetization","score_opus":0.007612188822517049,"score_gpt":0.21568452088467926,"score_spread":0.20807233206216222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2532278570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975235,0.000028015998,0.00180544,0.000020036188,0.0000032637388,0.000007369328,0.00007754832,0.000039685507,0.00049518095],"genre_scores_gemma":[0.9989378,0.0000104245855,0.00090724166,0.0000027471947,0.0000014204048,0.0000040054947,0.00008376099,0.000007728512,0.00004488716],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999193,0.00002729352,0.000006658137,0.000019683379,0.000012832928,0.000014143833],"domain_scores_gemma":[0.99934214,0.0003176593,0.00008148942,0.00008570075,0.000060853057,0.00011217702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028841087,0.00025434137,0.00040620237,0.0004325154,0.0003679505,0.0005106778,0.00051217637,0.00057199923,0.00080481416],"category_scores_gemma":[0.0018610336,0.00023746496,0.00040512206,0.0003783119,0.00036656772,0.00062764675,0.00055512,0.00035489126,0.0001260289],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001116853,0.00013064247,0.07195535,0.00003383459,0.000087491746,0.000085179316,0.00009801545,0.9188377,0.0049299067,0.00084504153,0.00012402183,0.0027611472],"study_design_scores_gemma":[0.000020516121,0.00007813505,0.018991983,0.0000029063938,0.000010983521,0.000023741923,0.000052678428,0.9788518,0.0012462903,0.0006066165,0.00010685288,0.0000075225244],"about_ca_topic_score_codex":0.0055227266,"about_ca_topic_score_gemma":0.0028026947,"teacher_disagreement_score":0.0055227266,"about_ca_system_score_codex":0.00046480657,"about_ca_system_score_gemma":0.00021628324,"threshold_uncertainty_score":0.0109811425},"labels":[],"label_agreement":null},{"id":"W2533579457","doi":"10.3847/1538-4357/834/1/57","title":"PHYSICAL PROPERTIES OF MOLECULAR CLOUDS FOR THE ENTIRE MILKY WAY DISK","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":382,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Molecular cloud; Milky Way; Galactic plane; Sigma; RADIUS; Velocity dispersion; Galaxy; Normalization (sociology); Astronomy; Stars","score_opus":0.012635560049910939,"score_gpt":0.23207512073882675,"score_spread":0.21943956068891582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2533579457","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981517,0.00022685208,0.00018891039,0.00001571521,0.0000020484918,0.000004632414,0.0010564044,0.000019027142,0.00033476116],"genre_scores_gemma":[0.9981615,0.000079747646,0.00016715482,0.000005550993,0.000004885075,0.0000044104613,0.0014925232,0.000005049723,0.00007929536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998049,0.000018720317,0.000017200993,0.000048734953,0.000059694972,0.00005071835],"domain_scores_gemma":[0.9986926,0.00027663202,0.00046815025,0.0001759217,0.000206009,0.0001808029],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037332164,0.0001705596,0.0003463201,0.0021877205,0.0003933809,0.0008519905,0.0003082878,0.00024875844,0.0008086471],"category_scores_gemma":[0.0021355909,0.00018753065,0.00026286612,0.0018828678,0.0001773862,0.0005383385,0.00046035962,0.00012667976,0.00025222255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000064526525,0.000025101563,0.9886131,0.000022730746,0.00007862839,0.00009040171,0.00009130209,0.0031124647,0.0032014844,0.00029304964,0.0003546934,0.004052401],"study_design_scores_gemma":[0.0000073377137,0.000022661834,0.99183744,0.0000072873277,0.000022429625,0.00011157621,0.00008186658,0.0061355573,0.00063358736,0.00018275851,0.0009526088,0.000004933317],"about_ca_topic_score_codex":0.005153564,"about_ca_topic_score_gemma":0.0041885697,"teacher_disagreement_score":0.005153564,"about_ca_system_score_codex":0.00039333553,"about_ca_system_score_gemma":0.00019898781,"threshold_uncertainty_score":0.010247111},"labels":[],"label_agreement":null},{"id":"W2533804033","doi":"10.3847/0004-637x/831/2/140","title":"OBSERVATIONS OF ROTATING RADIO TRANSIENTS WITH THE FIRST STATION OF THE LONG WAVELENGTH ARRAY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Physics; Dispersion (optics); Wavelength; Astrophysics; Pulse (music); Low frequency; Scattering; Interstellar medium; Astronomy; Optics","score_opus":0.015412613606036562,"score_gpt":0.2702102361823947,"score_spread":0.25479762257635813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2533804033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99769294,0.00013950463,0.00063999475,0.0000225572,0.0000064881087,0.0000085549,0.00043441993,0.000037051588,0.0010184563],"genre_scores_gemma":[0.99754226,0.00008305956,0.0009486374,0.000016016587,0.000022033373,0.000007592081,0.00081513386,0.000007621926,0.0005577499],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999778,0.000030953244,0.000009987204,0.00006359363,0.00005130606,0.00006622303],"domain_scores_gemma":[0.99906605,0.00021547228,0.00033378412,0.00009236853,0.00012675577,0.00016551426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030716037,0.00018434426,0.00025410962,0.0013103,0.00034308486,0.0004275206,0.00019055644,0.00026509378,0.0009748376],"category_scores_gemma":[0.0007287786,0.00012774224,0.00012634933,0.0007295569,0.00015653962,0.00027787648,0.0004113017,0.0003472112,0.00047749528],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044172045,0.00020296664,0.8373789,0.00007417852,0.00007039275,0.00041037786,0.00042086415,0.0007969833,0.120548494,0.00019669236,0.0006455177,0.038812928],"study_design_scores_gemma":[0.000012025288,0.00013266799,0.9926535,0.000007700193,0.000017237395,0.00030161324,0.000064553395,0.00058531616,0.005094133,0.00004405742,0.0010791403,0.000008062109],"about_ca_topic_score_codex":0.0011420873,"about_ca_topic_score_gemma":0.0018096019,"teacher_disagreement_score":0.0013103,"about_ca_system_score_codex":0.00018277674,"about_ca_system_score_gemma":0.00010315581,"threshold_uncertainty_score":0.003261149},"labels":[],"label_agreement":null},{"id":"W2535520888","doi":"10.3847/1538-4357/833/2/289","title":"ACCURATE POLARIZATION CALIBRATION AT 800 MHz WITH THE GREEN BANK TELESCOPE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; Canadian Institute for Advanced Research","funders":"","keywords":"Polarization (electrochemistry); Telescope; Green Bank Telescope; Synchrotron; Leakage (economics); Stokes parameters; Quasar","score_opus":0.008369022922367282,"score_gpt":0.20552156172988387,"score_spread":0.1971525388075166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2535520888","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8624627,0.00021329342,0.12199911,0.00014980271,0.000059864968,0.000102643295,0.0034546747,0.0017111768,0.009846763],"genre_scores_gemma":[0.8927584,0.00015321295,0.103359945,0.000117367745,0.000037763784,0.00012027704,0.002023456,0.00030216834,0.0011273586],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9992613,0.00013636207,0.000028199704,0.00021301697,0.00026857058,0.000092415314],"domain_scores_gemma":[0.99900997,0.00009620567,0.00022419402,0.00032988883,0.00027107412,0.00006865668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009355129,0.0002790587,0.00029366807,0.0009946442,0.000515529,0.0006096558,0.00041177624,0.00038802155,0.0017318769],"category_scores_gemma":[0.0012748246,0.00034334583,0.00020712039,0.0017234103,0.00035141534,0.0004000722,0.00071960775,0.00047669944,0.0011173083],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041343717,0.00013655025,0.24034376,0.00008018117,0.00013302425,0.00021781788,0.0005426248,0.00596817,0.6464083,0.0017619281,0.0028856401,0.101108626],"study_design_scores_gemma":[0.00008198874,0.0001874652,0.5815732,0.000042833297,0.00013231575,0.0006432846,0.00024359323,0.033306938,0.3655593,0.0014763712,0.016664056,0.000088624096],"about_ca_topic_score_codex":0.002794952,"about_ca_topic_score_gemma":0.0055757384,"teacher_disagreement_score":0.002794952,"about_ca_system_score_codex":0.00039147638,"about_ca_system_score_gemma":0.00038784734,"threshold_uncertainty_score":0.0057936907},"labels":[],"label_agreement":null},{"id":"W2536300955","doi":"10.3847/1538-4357/aa5f56","title":"Mass Distribution in Galaxy Cluster Cores","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Physics; Galaxy cluster; Astrophysics; Cluster (spacecraft); Galaxy; Mass distribution; Dark matter; Abell 2744; Brightest cluster galaxy; Galaxy groups and clusters; Astronomy","score_opus":0.008653067531202945,"score_gpt":0.22884794412584888,"score_spread":0.22019487659464593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2536300955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973814,0.00009104394,0.00013032604,0.000015314543,0.0000013193396,0.0000028230456,0.0006872948,0.000018741954,0.001671672],"genre_scores_gemma":[0.99934834,0.000017587772,0.000051661893,0.000003670817,0.0000018261992,0.0000013834698,0.0003555012,0.0000031101513,0.00021690171],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988294,0.000011687622,0.0000072294483,0.00004377134,0.000022862836,0.00003145521],"domain_scores_gemma":[0.9992262,0.00013911379,0.00019583048,0.000072234085,0.00021531372,0.00015120287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016461921,0.00012220803,0.00015789179,0.0013439851,0.0002116263,0.0006077254,0.00021263052,0.00013827096,0.0026739151],"category_scores_gemma":[0.0012954373,0.00008104404,0.00009969932,0.0006036323,0.00026037678,0.00024526424,0.00047591372,0.00008883754,0.00058600644],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019519516,0.000013224057,0.98430115,0.000021510747,0.00005923989,0.00006560398,0.0003341855,0.0014374428,0.0073823244,0.00097198074,0.0005056627,0.0047125374],"study_design_scores_gemma":[0.0000044202015,0.00003240182,0.9968004,0.000004188469,0.0000069587563,0.00007881233,0.00012864638,0.0012723646,0.0009351127,0.00026540202,0.00046585727,0.0000054780685],"about_ca_topic_score_codex":0.006160452,"about_ca_topic_score_gemma":0.005124519,"teacher_disagreement_score":0.006160452,"about_ca_system_score_codex":0.0003471323,"about_ca_system_score_gemma":0.00014707232,"threshold_uncertainty_score":0.012249172},"labels":[],"label_agreement":null},{"id":"W2539214099","doi":"10.3847/1538-4357/833/2/224","title":"STAR FORMATION IN INTERMEDIATE REDSHIFT 0.2 &lt; z &lt; 0.7 BRIGHTEST CLUSTER GALAXIES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Star formation; Astronomy; Galaxy; Stellar mass; Redshift; Galaxy cluster","score_opus":0.00665881700701278,"score_gpt":0.20560126999790282,"score_spread":0.19894245299089003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2539214099","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99983704,0.000014877385,0.000008888252,0.0000034928596,2.9032464e-7,6.2295913e-7,0.00004772778,0.0000013034883,0.000085791944],"genre_scores_gemma":[0.9998363,0.0000058511314,0.000013182194,0.0000021548751,0.0000010598856,5.195988e-7,0.00009174461,5.150521e-7,0.000048621772],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984086,0.00001930167,0.000007815927,0.000039711034,0.000024688836,0.00006751525],"domain_scores_gemma":[0.99921596,0.000061088984,0.00022676779,0.000052509742,0.00010535881,0.00033822493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026182184,0.00014448122,0.00022282879,0.001296707,0.00038758214,0.00050459197,0.00017962746,0.00016642381,0.0010876008],"category_scores_gemma":[0.00053022796,0.00010135488,0.00015003284,0.00053565623,0.0003945382,0.00019006523,0.00043169098,0.0001338525,0.00022934418],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000069213274,0.000018470915,0.9971154,0.000001950632,0.000008196067,0.000030864303,0.00015809087,0.000028055112,0.001928414,0.000026494852,0.00004028356,0.0005744914],"study_design_scores_gemma":[7.195545e-7,0.000010312044,0.9997967,3.2454116e-7,0.0000017922584,0.000017031254,0.000051289066,0.000023418512,0.00007093913,0.0000035555317,0.000023553415,4.5601038e-7],"about_ca_topic_score_codex":0.011836092,"about_ca_topic_score_gemma":0.013037212,"teacher_disagreement_score":0.011836092,"about_ca_system_score_codex":0.00030610384,"about_ca_system_score_gemma":0.00015711415,"threshold_uncertainty_score":0.023534358},"labels":[],"label_agreement":null},{"id":"W2539694342","doi":"10.3847/1538-4357/833/2/213","title":"DELAY SPECTRUM WITH PHASE-TRACKING ARRAYS: EXTRACTING THE H i POWER SPECTRUM FROM THE EPOCH OF REIONIZATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; LOFAR; Physics; HERA; Interferometry; SIGNAL (programming language); Spectral density; Redshift; Pipeline (software); Computer science; Tracking (education); Radio telescope; Astrophysics; Optics; Telecommunications; Galaxy","score_opus":0.010821545613246783,"score_gpt":0.2322698085567637,"score_spread":0.22144826294351694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2539694342","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6773521,0.00026683154,0.31828117,0.000102537466,0.000030737014,0.00005126846,0.00047734124,0.0012155693,0.0022225077],"genre_scores_gemma":[0.81630266,0.00013599133,0.18235204,0.000036803318,0.000034299428,0.00003259232,0.0004789726,0.00012623213,0.00050034595],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999049,0.000017689741,0.00000385127,0.000030322873,0.000029929673,0.000013393141],"domain_scores_gemma":[0.9997801,0.000066224246,0.000067858164,0.00003778573,0.000028711509,0.000019387608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003150396,0.0004561117,0.00018665758,0.00087366067,0.00013929763,0.00041155372,0.00041326784,0.00027466146,0.00057853403],"category_scores_gemma":[0.0006435694,0.00020182169,0.00035734638,0.0007533916,0.00017200825,0.00054866483,0.00029593112,0.00030314678,0.00023081417],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005068644,0.00020162624,0.089834,0.00015818389,0.0002658055,0.00032119616,0.0002526583,0.110093735,0.56253034,0.0035383392,0.00092944293,0.23136774],"study_design_scores_gemma":[0.00004910533,0.00019234039,0.113843866,0.000016030728,0.000080827755,0.00027881443,0.00009180235,0.7668005,0.112873904,0.0030572622,0.002646057,0.000069531314],"about_ca_topic_score_codex":0.0011610178,"about_ca_topic_score_gemma":0.0017658301,"teacher_disagreement_score":0.0011610178,"about_ca_system_score_codex":0.00019901569,"about_ca_system_score_gemma":0.00021380394,"threshold_uncertainty_score":0.0023085475},"labels":[],"label_agreement":null},{"id":"W2540911620","doi":"10.3847/1538-4357/835/2/273","title":"Intensity Mapping of Hα, Hβ, , and Lines at z &lt; 5","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Intensity mapping; Intensity (physics); Galaxy; Hydrogen line; Emission spectrum; Spectral line; Line (geometry); Luminosity","score_opus":0.013414040388078132,"score_gpt":0.22209788985279805,"score_spread":0.2086838494647199,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2540911620","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99415004,0.000025103966,0.003753015,0.000018636107,0.0000018718387,0.0000038300172,0.00037475643,0.000086602035,0.0015862058],"genre_scores_gemma":[0.9977532,0.000008514784,0.0016818322,0.0000051008537,0.0000024388607,0.0000020909758,0.00033258848,0.000008881408,0.00020530181],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999212,0.000008865464,0.000001862056,0.000021819995,0.000024789086,0.000021402366],"domain_scores_gemma":[0.99972004,0.000058419453,0.000099212346,0.000026677977,0.00005733855,0.000038345093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021579071,0.00019470282,0.00008750283,0.00046813145,0.00013407477,0.00021909837,0.00027332138,0.00013401674,0.0011740375],"category_scores_gemma":[0.00054427655,0.00007945526,0.00013058836,0.0002985832,0.0001428023,0.00023097706,0.00017817614,0.00013119858,0.00015643622],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018852536,0.000069593116,0.87892115,0.000026522073,0.00009686598,0.00017504937,0.00007457463,0.022820925,0.06617708,0.0019188861,0.00094207807,0.02858877],"study_design_scores_gemma":[0.0000107451915,0.000031096693,0.90387404,0.0000045004276,0.000027202856,0.000079168036,0.000052160016,0.07193862,0.022402959,0.000646252,0.000922369,0.000010911365],"about_ca_topic_score_codex":0.0059928037,"about_ca_topic_score_gemma":0.005005366,"teacher_disagreement_score":0.0059928037,"about_ca_system_score_codex":0.00021597084,"about_ca_system_score_gemma":0.000100822006,"threshold_uncertainty_score":0.011915863},"labels":[],"label_agreement":null},{"id":"W2543636112","doi":"10.3847/0004-637x/831/1/46","title":"A MAGNETIC RIBBON MODEL FOR STAR-FORMING FILAMENTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Magnetic field; Ribbon; Molecular cloud; Ambipolar diffusion; Turbulence; Magnetohydrodynamics; Thermal; Projection (relational algebra)","score_opus":0.015813293698539045,"score_gpt":0.2461313315300268,"score_spread":0.23031803783148777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2543636112","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47912216,0.0012028132,0.40498284,0.0019106877,0.00022752372,0.000112712034,0.00058166694,0.000897442,0.1109621],"genre_scores_gemma":[0.9787992,0.00027708383,0.011307241,0.00010533839,0.00004779575,0.000063938016,0.00010714386,0.00008149769,0.009210676],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992037,0.00002005765,0.0000025386375,0.000014816549,0.000018884064,0.000023462879],"domain_scores_gemma":[0.9998,0.00003827954,0.00004382907,0.00002105141,0.00003958441,0.000057265373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016751788,0.00032265452,0.00037749502,0.00043849784,0.0007486698,0.000986206,0.00092097244,0.0013617338,0.0037577283],"category_scores_gemma":[0.00054330315,0.00024513167,0.0005158861,0.0002867562,0.00066294504,0.0009102014,0.0004981048,0.00045199113,0.0005798471],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008244473,0.000042948664,0.0011660577,0.000027730137,0.000021844156,0.000520854,0.00008729591,0.8280777,0.0101861395,0.1564544,0.0011408266,0.002191761],"study_design_scores_gemma":[0.000018789915,0.00001366676,0.00023534268,0.000005440624,0.000002988942,0.00005046135,0.000014350644,0.98503417,0.00029351562,0.013339208,0.0009847855,0.0000072502535],"about_ca_topic_score_codex":0.005065318,"about_ca_topic_score_gemma":0.002173032,"teacher_disagreement_score":0.005065318,"about_ca_system_score_codex":0.00093825243,"about_ca_system_score_gemma":0.00038574298,"threshold_uncertainty_score":0.012570798},"labels":[],"label_agreement":null},{"id":"W2543679060","doi":"10.3847/1538-4357/834/1/1","title":"DOES A DIFFERENTIATED, CARBONATE-RICH, ROCKY OBJECT POLLUTE THE WHITE DWARF SDSS J104341.53+085558.2?","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Spectral line; Spectrograph; Photosphere; Parent body; Spectroscopy; Planetesimal; Asteroid","score_opus":0.0070224855761297465,"score_gpt":0.2056346930478913,"score_spread":0.19861220747176156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2543679060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99915445,0.00008540532,0.00007205064,0.00003379597,0.0000045124634,0.0000022774252,0.00015476311,0.000011110239,0.00048166513],"genre_scores_gemma":[0.9990897,0.000049423576,0.00013270644,0.000048692706,0.000012724647,0.0000016592229,0.00042356513,0.000007089522,0.00023440695],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998411,0.00000753475,0.000014670725,0.00005494137,0.000038565133,0.00004307034],"domain_scores_gemma":[0.9994412,0.00003407835,0.00029803725,0.000045404253,0.000051313094,0.000129815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021956093,0.00035097203,0.00047847873,0.001069514,0.000584743,0.0009616136,0.00033334392,0.00046391334,0.0016903888],"category_scores_gemma":[0.00037611747,0.00022970462,0.00023714661,0.00089901115,0.00055200123,0.00043324125,0.0006015925,0.00018910787,0.0005116389],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018247601,0.000026944284,0.96640956,0.00005150144,0.00008995649,0.0006333013,0.00023604603,0.00016483196,0.028206762,0.00015592364,0.00027353395,0.0035691601],"study_design_scores_gemma":[0.0000063333746,0.000026331241,0.99729013,0.00000566286,0.000026966905,0.00021352801,0.00026039456,0.0002337842,0.0011616339,0.000056789522,0.00071397325,0.0000044724125],"about_ca_topic_score_codex":0.006825432,"about_ca_topic_score_gemma":0.011881644,"teacher_disagreement_score":0.006825432,"about_ca_system_score_codex":0.0005192207,"about_ca_system_score_gemma":0.00015169737,"threshold_uncertainty_score":0.013571441},"labels":[],"label_agreement":null},{"id":"W2545435752","doi":"10.3847/1538-4357/833/2/204","title":"THE FRAGMENTATION AND STABILITY OF HIERARCHICAL STRUCTURE IN SERPENS SOUTH","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Serpens; Fragmentation (computing); Astrophysics; Physics; Molecular cloud; Virial theorem; Virial mass; Cluster (spacecraft); Magnetic field; Star formation; Telescope; Stars; Galaxy","score_opus":0.008011670997169347,"score_gpt":0.23130886245355797,"score_spread":0.22329719145638863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2545435752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993351,0.00002339587,0.000059110804,0.0000056807853,6.435997e-7,0.0000013211137,0.00005307691,0.00000517452,0.0005164649],"genre_scores_gemma":[0.99969125,0.000019343483,0.000073530115,0.0000032839368,9.052884e-7,7.237136e-7,0.000102504484,0.0000020131147,0.0001063988],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999472,0.0000047140256,0.000002445217,0.000018657654,0.0000114419645,0.000015492244],"domain_scores_gemma":[0.9997968,0.000019534607,0.00010371967,0.000015547457,0.000025344667,0.00003908299],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006533716,0.00013944568,0.00011418705,0.0009844989,0.00028370993,0.00042860722,0.00016619924,0.00011311503,0.0009365313],"category_scores_gemma":[0.00030799813,0.00008947032,0.00012538365,0.00033908046,0.00043219142,0.00019027393,0.00037692237,0.0001238,0.00020107279],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024060393,0.000024374847,0.9026023,0.000036064805,0.000046791472,0.0011337769,0.0010463375,0.0018028619,0.08138696,0.00082728395,0.00018878051,0.01066398],"study_design_scores_gemma":[0.0000039056326,0.000021884274,0.99508625,0.000007033907,0.0000061424303,0.00033874004,0.00045033175,0.0009264914,0.0024327086,0.0002166287,0.0005060481,0.0000037956627],"about_ca_topic_score_codex":0.004974683,"about_ca_topic_score_gemma":0.005930282,"teacher_disagreement_score":0.004974683,"about_ca_system_score_codex":0.00040473798,"about_ca_system_score_gemma":0.00013557999,"threshold_uncertainty_score":0.00989145},"labels":[],"label_agreement":null},{"id":"W2546399365","doi":"10.3847/1538-4357/833/1/75","title":"A MONTE CARLO STUDY OF FLUX RATIOS OF RAMAN SCATTERED O vi FEATURES AT 6825 AND 7082 Å IN SYMBIOTIC STARS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Raman spectroscopy; Flux (metallurgy); Stars; Monte Carlo method; Rayleigh scattering; Spectral line; Raman scattering; Line (geometry)","score_opus":0.008866512199819574,"score_gpt":0.2207924325034399,"score_spread":0.21192592030362034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2546399365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939997,0.000053405503,0.0048373407,0.000053571548,0.0000040645837,0.000010823262,0.0000737422,0.000059913003,0.00090737425],"genre_scores_gemma":[0.9977598,0.000014046123,0.001928483,0.0000111197505,0.0000026045334,0.000011947582,0.00011530905,0.000011373335,0.00014525959],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997445,0.00010755539,0.0000097850325,0.000048439448,0.000044081917,0.000045672557],"domain_scores_gemma":[0.99478817,0.0041099554,0.0004157605,0.0002068513,0.00027641092,0.00020282374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013224126,0.00028509524,0.00033531914,0.0007056147,0.00056487304,0.0005499694,0.0008038469,0.0008554135,0.0009467875],"category_scores_gemma":[0.0044324226,0.0004000905,0.00054794864,0.0004560387,0.0005060068,0.00045649623,0.00025027,0.00046584147,0.00007528826],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024875705,0.00011310573,0.04036355,0.00002664688,0.00010893176,0.00024309124,0.000059057318,0.948058,0.0044336016,0.003800856,0.00022388913,0.0023204414],"study_design_scores_gemma":[0.00001716859,0.000040343282,0.0065698987,0.0000039121164,0.0000128047495,0.00004762608,0.00001662996,0.9919117,0.00096082577,0.00033791954,0.0000705908,0.000010559604],"about_ca_topic_score_codex":0.011255233,"about_ca_topic_score_gemma":0.0055919266,"teacher_disagreement_score":0.011255233,"about_ca_system_score_codex":0.00093527307,"about_ca_system_score_gemma":0.00042869346,"threshold_uncertainty_score":0.022379458},"labels":[],"label_agreement":null},{"id":"W2546754458","doi":"10.3847/1538-4357/836/1/130","title":"Alma Observations of Massive Molecular Gas Filaments Encasing Radio Bubbles in the Phoenix Cluster","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Cluster (spacecraft); Quasar; Galaxy cluster; Star formation; Galaxy; Solar mass; Cooling flow; X-shaped radio galaxy; Phoenix; Molecular cloud","score_opus":0.022507161752667777,"score_gpt":0.2655964990360737,"score_spread":0.2430893372834059,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2546754458","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981901,0.000058913094,0.00025100328,0.000029494226,0.0000031681138,0.000008171004,0.00025530008,0.00005549668,0.001148237],"genre_scores_gemma":[0.99897826,0.000025194273,0.00042682877,0.000016125348,0.00000808385,0.0000061452147,0.00020235586,0.0000058123155,0.0003313258],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999373,0.0000026477192,0.0000014729878,0.00002396071,0.000016378552,0.000018299865],"domain_scores_gemma":[0.9998386,0.000014655027,0.00004521619,0.000016646438,0.000023613891,0.000061352606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012237571,0.00016609103,0.00013197263,0.00065738894,0.00040671226,0.00038736127,0.00029947297,0.0002070426,0.0010400104],"category_scores_gemma":[0.00019926025,0.00013302114,0.000110993446,0.00026581812,0.00019223246,0.0001979402,0.00049570604,0.00030288793,0.00020503641],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077754346,0.00013916033,0.5853807,0.000054161213,0.00014671776,0.0015014847,0.0010367394,0.0011686685,0.39334553,0.00036886567,0.0016275969,0.014452831],"study_design_scores_gemma":[0.000026417372,0.00006798724,0.986408,0.000005649338,0.000029865798,0.0002715219,0.00016109216,0.0017547087,0.009260697,0.000064577645,0.0019394933,0.000010009515],"about_ca_topic_score_codex":0.009694513,"about_ca_topic_score_gemma":0.010315609,"teacher_disagreement_score":0.009694513,"about_ca_system_score_codex":0.00032549602,"about_ca_system_score_gemma":0.00008750124,"threshold_uncertainty_score":0.019276202},"labels":[],"label_agreement":null},{"id":"W2547056004","doi":"10.3847/0004-637x/831/2/130","title":"GAS-PHASE ABSORPTIONS OF C<sup>+</sup> <sub>60</sub>: A NEW COMPARISON WITH ASTRONOMICAL MEASUREMENTS*†","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Astronomy; Nuclear physics; Atomic physics","score_opus":0.026956807669608143,"score_gpt":0.26463391076810233,"score_spread":0.23767710309849419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2547056004","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900385,0.001585104,0.0026387013,0.0000777299,0.00004707539,0.000010116019,0.00028549143,0.00010872261,0.0052084904],"genre_scores_gemma":[0.9965448,0.0003534793,0.0021718107,0.00005511357,0.00002773725,0.000010215004,0.00031930997,0.000033219178,0.00048448142],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997949,0.000020416292,0.000008380979,0.00008545567,0.00005914454,0.00003173336],"domain_scores_gemma":[0.99967194,0.00006456151,0.000088638844,0.00005868064,0.00007111552,0.000045036824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002743223,0.00021093655,0.00017520048,0.00079032074,0.0004736913,0.0006918777,0.00028639662,0.00048056996,0.0035885812],"category_scores_gemma":[0.00048333622,0.00009972926,0.00011857273,0.0005223097,0.0004862334,0.00038522392,0.0006462581,0.00039563514,0.0005367591],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035470983,0.00008039675,0.0367304,0.000092055765,0.000029116442,0.000072904724,0.00012406007,0.00009125797,0.94152856,0.0008800201,0.00071880483,0.01929789],"study_design_scores_gemma":[0.00003651808,0.000211811,0.3084323,0.000024091993,0.00008707284,0.00081107,0.00023225645,0.0018249876,0.67466205,0.00071809685,0.012926829,0.000032800686],"about_ca_topic_score_codex":0.001334774,"about_ca_topic_score_gemma":0.0016907034,"teacher_disagreement_score":0.0035885812,"about_ca_system_score_codex":0.00038503922,"about_ca_system_score_gemma":0.00013236028,"threshold_uncertainty_score":0.012005031},"labels":[],"label_agreement":null},{"id":"W2547121134","doi":"10.3847/1538-4357/836/1/120","title":"The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to ∼10<sup>6</sup> L<sub>⊙</sub> and Comparisons with Galaxy Formation Models","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Waterloo; Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Virgo Cluster; Galaxy; Photometry (optics); Galaxy formation and evolution; Brightest cluster galaxy; Flattening; Galaxy cluster; Milky Way","score_opus":0.04615631335751557,"score_gpt":0.24626825872588418,"score_spread":0.2001119453683686,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2547121134","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.891963,0.0006052843,0.001239907,0.0004603557,0.000045841683,0.000057887723,0.083857834,0.00033090857,0.021439072],"genre_scores_gemma":[0.8863109,0.00025233885,0.0020409033,0.00016648624,0.00002445646,0.0000557708,0.10283549,0.00009410475,0.008219594],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990594,0.000012570983,0.000003402759,0.00002654064,0.00002333686,0.000028089125],"domain_scores_gemma":[0.99979764,0.000015115975,0.000044531906,0.000028364655,0.00003858851,0.000075686345],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022611959,0.00014928365,0.00010743129,0.0008356124,0.00021712501,0.00040516842,0.00026243817,0.0001628185,0.0036201475],"category_scores_gemma":[0.00039398496,0.00008103291,0.00019881067,0.00082705996,0.00012184976,0.00018034189,0.00035843,0.00015498755,0.0017262035],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031623026,0.0000843064,0.8919286,0.00011150382,0.00008098887,0.00013913726,0.00043750284,0.0025377523,0.005130932,0.0028137947,0.047523122,0.048896167],"study_design_scores_gemma":[0.0000056779913,0.000009890635,0.9876579,0.000007904679,0.000007975183,0.000025712576,0.00007117048,0.00075108843,0.00034878726,0.00023560437,0.010874383,0.000004005549],"about_ca_topic_score_codex":0.054791555,"about_ca_topic_score_gemma":0.06719258,"teacher_disagreement_score":0.054791555,"about_ca_system_score_codex":0.0006292036,"about_ca_system_score_gemma":0.00027508996,"threshold_uncertainty_score":0.10894531},"labels":[],"label_agreement":null},{"id":"W2547249076","doi":"10.3847/1538-4357/833/2/233","title":"AN EXPLORATION OF THE STATISTICAL SIGNATURES OF STELLAR FEEDBACK","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Computer science; Astronomy; Psychology; Physics","score_opus":0.016078276185125542,"score_gpt":0.2570655976420016,"score_spread":0.24098732145687607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2547249076","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968368,0.000013040334,0.0025280109,0.0000474435,0.0000025080337,0.0000037222906,0.00012736657,0.00006067266,0.0003803637],"genre_scores_gemma":[0.99959916,0.0000029746896,0.00030687772,0.0000030695144,0.0000014213495,0.0000012137289,0.00006274389,0.000004094093,0.00001846605],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99983025,0.000061717226,0.000008543615,0.00003732801,0.000040353312,0.000021649954],"domain_scores_gemma":[0.9968154,0.0018944436,0.00059962715,0.00028001197,0.00023794675,0.0001726661],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077160785,0.00016562767,0.0001879721,0.0006865305,0.00021834945,0.0005409786,0.00025061241,0.0002520925,0.0005658226],"category_scores_gemma":[0.0041351933,0.00010380966,0.00024740005,0.0004216129,0.00050192775,0.0003505873,0.00029982638,0.00024115945,0.000044813572],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028966088,0.00020728915,0.34178662,0.000051941824,0.00014752608,0.0002201917,0.00018220721,0.6161961,0.018299535,0.009812788,0.00079873845,0.012007366],"study_design_scores_gemma":[0.0000132446185,0.00008663187,0.09100834,0.00000462218,0.000010822165,0.000045218145,0.000056034653,0.903057,0.0026261248,0.0028925224,0.000183296,0.000016190266],"about_ca_topic_score_codex":0.002615986,"about_ca_topic_score_gemma":0.0018462709,"teacher_disagreement_score":0.002615986,"about_ca_system_score_codex":0.0003870215,"about_ca_system_score_gemma":0.00023981761,"threshold_uncertainty_score":0.0052015185},"labels":[],"label_agreement":null},{"id":"W2547377462","doi":"10.3847/1538-4357/834/1/20","title":"SPECTRAL ENERGY DISTRIBUTION MAPPING OF TWO ELLIPTICAL GALAXIES ON SUB-kpc SCALES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Princeton University","keywords":"Physics; Astrophysics; Galaxy; Elliptical galaxy; Metallicity; Luminous infrared galaxy; Star formation; Stellar population; Surface brightness fluctuation; Spectral energy distribution; Stellar mass; Stars; Astronomy; Population; Disc galaxy; Medicine","score_opus":0.0075720596501517206,"score_gpt":0.20659294859818192,"score_spread":0.1990208889480302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2547377462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982869,0.00004616425,0.00044100801,0.0000115574285,0.0000011069611,0.0000030293113,0.00035946857,0.000058423455,0.00079241063],"genre_scores_gemma":[0.99861455,0.000017048422,0.0006721662,0.0000041136213,0.0000023939135,0.0000017134394,0.0005102009,0.0000072926355,0.00017056172],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999317,0.0000054975358,0.0000027347437,0.000028742794,0.000014735099,0.000016488324],"domain_scores_gemma":[0.9996538,0.00006892931,0.00008091088,0.000052942047,0.00006534585,0.00007812353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000115818475,0.00013356678,0.00013601506,0.001272235,0.00014418438,0.0003320612,0.00018517718,0.00013719377,0.001093558],"category_scores_gemma":[0.0003141662,0.00010530137,0.00019084901,0.00048681817,0.00012775735,0.00015328897,0.00027392872,0.00009989059,0.00024748122],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038305862,0.00014263939,0.8801599,0.000053367487,0.000137201,0.00056049135,0.00032575216,0.0068584383,0.08786735,0.00089809136,0.0006598142,0.021953778],"study_design_scores_gemma":[0.000007234058,0.000017918388,0.98661566,0.000003117374,0.000017092303,0.000112199574,0.000074994925,0.0074425647,0.0048230807,0.000096816664,0.00078384794,0.0000053773265],"about_ca_topic_score_codex":0.0037995095,"about_ca_topic_score_gemma":0.003690252,"teacher_disagreement_score":0.0037995095,"about_ca_system_score_codex":0.0003280409,"about_ca_system_score_gemma":0.000062156265,"threshold_uncertainty_score":0.0075547695},"labels":[],"label_agreement":null},{"id":"W2548181745","doi":"10.3847/1538-4357/834/2/210","title":"VLT/MAGELLAN SPECTROSCOPY OF 29 STRONG LENSING SELECTED GALAXY CLUSTERS","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Redshift; Velocity dispersion; Galaxy cluster; Galaxy; Weak gravitational lensing; Gravitational lens; Cluster (spacecraft); Strong gravitational lensing; Redshift survey","score_opus":0.009737541850432947,"score_gpt":0.2342331872104052,"score_spread":0.22449564535997227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2548181745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994814,0.00003292578,0.00006234935,0.0000056691674,7.1357044e-7,0.0000034610703,0.00023850806,0.0000119675105,0.00016313848],"genre_scores_gemma":[0.998657,0.000020813724,0.00022663102,0.0000073904903,0.0000043298783,0.0000042302263,0.0008818391,0.0000047536273,0.00019305723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996792,0.0000346545,0.000015330908,0.000099966564,0.00008829661,0.00008254768],"domain_scores_gemma":[0.99910694,0.0001166776,0.00023091525,0.0001138924,0.00012708537,0.0003044485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044478846,0.000305307,0.00030217695,0.001981286,0.0006062268,0.00042942906,0.0004322483,0.00021536238,0.0010130077],"category_scores_gemma":[0.0008102854,0.00015619458,0.00019642278,0.0011287186,0.00028398866,0.00018453402,0.0008492408,0.00015702577,0.0002698203],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023990427,0.00006690163,0.9630365,0.000028699927,0.00008772928,0.00028627203,0.00049733574,0.0008721974,0.026504979,0.00012543816,0.0005349245,0.0077190506],"study_design_scores_gemma":[0.000008756703,0.000073034724,0.9965288,0.0000022396225,0.000011967121,0.00009404436,0.00012002262,0.00069519266,0.0019311368,0.00001977513,0.0005096871,0.000005517266],"about_ca_topic_score_codex":0.012358988,"about_ca_topic_score_gemma":0.021356666,"teacher_disagreement_score":0.012358988,"about_ca_system_score_codex":0.00063861936,"about_ca_system_score_gemma":0.00029097695,"threshold_uncertainty_score":0.024574101},"labels":[],"label_agreement":null},{"id":"W2550898223","doi":"10.3847/0004-637x/832/1/68","title":"THE ORBIT, ROTATION, AND GRANULATION OF THE G7 GIANT β Her","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Line (geometry); Radial velocity; Flux (metallurgy); Spectral line; Light curve; Rotation (mathematics); Dispersion (optics); Granulation; Absolute magnitude; Optics; Geometry; Astronomy; Stars; Classical mechanics","score_opus":0.0071266425357124595,"score_gpt":0.20806739756284368,"score_spread":0.2009407550271312,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2550898223","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994636,0.000027220423,0.000021600157,0.000006311925,5.8469954e-7,7.312167e-7,0.000050111263,0.000004189898,0.0004256113],"genre_scores_gemma":[0.99965227,0.000015727626,0.000031760745,0.00000602746,0.0000018921368,9.109959e-7,0.0001780559,0.0000048102556,0.000108409215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995255,0.000005797408,0.0000022993695,0.000015141605,0.000010285186,0.000014035678],"domain_scores_gemma":[0.9997491,0.000032526408,0.00010600033,0.00002320699,0.00002795112,0.00006112491],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011323935,0.00014500237,0.00021025845,0.00089527736,0.00033827696,0.00053726515,0.00014241325,0.00020604926,0.0007068228],"category_scores_gemma":[0.00032884596,0.0001181256,0.00009473007,0.00045558097,0.00035874007,0.00018651204,0.00033158768,0.00014351391,0.00034019025],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007174869,0.000059647766,0.86260885,0.0000321813,0.00005020269,0.00063996005,0.0006364115,0.0006263274,0.12217211,0.00036804125,0.00042372604,0.011665009],"study_design_scores_gemma":[0.000005577923,0.000054074557,0.9977375,0.0000028129366,0.0000067238075,0.00018554648,0.00014077612,0.0005581885,0.00093181693,0.000078173245,0.00029546308,0.00000327861],"about_ca_topic_score_codex":0.0023124954,"about_ca_topic_score_gemma":0.003262417,"teacher_disagreement_score":0.0023124954,"about_ca_system_score_codex":0.0002782044,"about_ca_system_score_gemma":0.000074731404,"threshold_uncertainty_score":0.0045980215},"labels":[],"label_agreement":null},{"id":"W2552708734","doi":"10.3847/1538-4357/aa6c47","title":"Search for Gravitational Waves Associated with Gamma-Ray Bursts during the First Advanced LIGO Observing Run and Implications for the Origin of GRB 150906B","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Royal Society; Ministerio de Economía y Competitividad; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Fundação de Amparo à Pesquisa do Estado de São Paulo; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; European Commission; Russian Foundation for Basic Research; Leverhulme Trust; Scottish Funding Council; Scottish Universities Physics Alliance; Hungarian Scientific Research Fund; Science and Engineering Research Board; National Science Foundation; Istituto Nazionale di Fisica Nucleare; Kavli Foundation; National Aeronautics and Space Administration","keywords":"Physics; LIGO; Gamma-ray burst; Gravitational wave; Astrophysics; Neutron star; Galaxy; Black hole (networking); Astronomy; Luminosity; Observatory","score_opus":0.022899375608721954,"score_gpt":0.2798818646927756,"score_spread":0.25698248908405363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2552708734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987507,0.00008919369,0.00019967591,0.00005309096,0.0000035424416,0.0000040371274,0.0003368813,0.000018412127,0.00054434995],"genre_scores_gemma":[0.9988667,0.000032588636,0.00018115375,0.000025170806,0.0000076087395,0.0000042040892,0.000759284,0.000006541371,0.00011676996],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994342,0.000102923375,0.000047798403,0.00012541535,0.00015958941,0.00013019622],"domain_scores_gemma":[0.9955664,0.00086213654,0.0020817376,0.00031841712,0.0003296795,0.0008415313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00097429677,0.0002894679,0.00048124586,0.0020887046,0.0004975209,0.0011819189,0.0002953446,0.0005015093,0.0010843276],"category_scores_gemma":[0.0029222812,0.000153181,0.00043435692,0.0008596388,0.0003950502,0.00038191982,0.0009771,0.00048393782,0.00032811068],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019977777,0.000054467753,0.98818564,0.0000115466855,0.000054740256,0.00015188946,0.00010181071,0.00023478548,0.007057517,0.00010220567,0.00014673667,0.0036989006],"study_design_scores_gemma":[0.000007662132,0.00006568195,0.9981158,0.000007632217,0.000024575238,0.0001597845,0.000090310525,0.0004431828,0.00077704526,0.00006231091,0.00023888466,0.0000071314785],"about_ca_topic_score_codex":0.0034665074,"about_ca_topic_score_gemma":0.0041901334,"teacher_disagreement_score":0.0034665074,"about_ca_system_score_codex":0.00031096724,"about_ca_system_score_gemma":0.00020794437,"threshold_uncertainty_score":0.006892681},"labels":[],"label_agreement":null},{"id":"W2553309653","doi":"10.3847/1538-4357/834/1/2","title":"A SEARCH FOR SPECTRAL HYSTERESIS AND ENERGY-DEPENDENT TIME LAGS FROM X-RAY AND TeV GAMMA-RAY OBSERVATIONS OF Mrk 421","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Japan Society for the Promotion of Science; Office of Science; Instituto de Astrofísica de Canarias; Hrvatska Zaklada za Znanost; Bundesministerium für Bildung und Forschung; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Leicester; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; European Regional Development Fund; U.S. Department of Energy; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; NASA Headquarters; National Science Foundation","keywords":"Blazar; Spectral index; Spectral density; Flare; Broadband; Spectral line; RADIUS; Synchrotron; Spectral shape analysis","score_opus":0.0145436042285864,"score_gpt":0.21873827424803224,"score_spread":0.20419467001944586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2553309653","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984505,0.00014103294,0.00033739614,0.000037464568,0.0000028332931,0.0000038132384,0.0001456528,0.000031875097,0.00084936654],"genre_scores_gemma":[0.9991416,0.000044562912,0.0003369616,0.000016945769,0.000007409917,0.0000032718585,0.00029487885,0.000008883118,0.00014554289],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998963,0.000008586001,0.000007364995,0.00003810024,0.000026567428,0.000022988179],"domain_scores_gemma":[0.99934906,0.00007934171,0.0003160174,0.000053337855,0.000060532584,0.00014162937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024336741,0.00016841362,0.00020230237,0.0008465585,0.0002956996,0.00059439323,0.00024247571,0.00029380948,0.0010435028],"category_scores_gemma":[0.00053042965,0.00023232085,0.000196464,0.00047301291,0.0001802946,0.00029784854,0.00054812984,0.0003445801,0.00019795059],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031915802,0.00009909998,0.84811705,0.00008019891,0.00015945443,0.000559837,0.0005108538,0.0007565985,0.13532564,0.00031440193,0.00037716233,0.013380596],"study_design_scores_gemma":[0.0000058151904,0.000035179655,0.9967519,0.0000053032054,0.000017415226,0.0002113781,0.00007630562,0.0006066677,0.0018359139,0.00004502826,0.00040451283,0.000004716291],"about_ca_topic_score_codex":0.0010657249,"about_ca_topic_score_gemma":0.002399527,"teacher_disagreement_score":0.0010657249,"about_ca_system_score_codex":0.00016143154,"about_ca_system_score_gemma":0.00014655113,"threshold_uncertainty_score":0.0034908652},"labels":[],"label_agreement":null},{"id":"W2555513711","doi":"10.3847/1538-4357/835/1/65","title":"SPACE TELESCOPE AND OPTICAL REVERBERATION MAPPING PROJECT.VI. REVERBERATING DISK MODELS FOR NGC 5548","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Natural Sciences and Engineering Research Council of Canada; University of California, Santa Barbara; Jet Propulsion Laboratory; National Research Foundation of Korea; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; American Academy in Rome; Science and Technology Facilities Council; National Research Foundation; Howard Hughes Medical Institute; Danmarks Grundforskningsfond; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Georgia State University; National Aeronautics and Space Administration; California Institute of Technology; Ministry of Science, ICT and Future Planning; Ohio State University; Danmarks Frie Forskningsfond; National Science Foundation","keywords":"Light curve; Accretion disc; Black-body radiation; Reverberation mapping; Galaxy; Accretion (finance); Spectral line; Active galactic nucleus","score_opus":0.03512551260643967,"score_gpt":0.2741752913174368,"score_spread":0.2390497787109971,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2555513711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98597187,0.00014196828,0.008815041,0.00022376403,0.000016112608,0.000031126092,0.0017314255,0.00024062968,0.0028280276],"genre_scores_gemma":[0.9943222,0.000058535563,0.0033134334,0.000028143719,0.000019342546,0.000024057084,0.0008864281,0.000066572014,0.001281321],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999941,0.000019261857,0.0000027979515,0.0000180173,0.00000674425,0.000012162654],"domain_scores_gemma":[0.99974626,0.000064857166,0.00006557939,0.000045750323,0.00003297677,0.000044509838],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036952583,0.00044312383,0.00032360523,0.00058490573,0.000243421,0.00043907342,0.0010800996,0.000602305,0.0028119376],"category_scores_gemma":[0.0010833999,0.00022530655,0.000554551,0.00029997018,0.00017737014,0.0005245929,0.0003544715,0.00029117955,0.0005108446],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026862643,0.00017767726,0.07952331,0.000053033018,0.00010879106,0.0005733116,0.00025313548,0.89275146,0.0043176273,0.0053388854,0.004422739,0.012211329],"study_design_scores_gemma":[0.000050802064,0.000027174603,0.013194614,0.0000049328046,0.000012500167,0.00006372438,0.000033854834,0.98346394,0.00018931393,0.0022350214,0.0007126977,0.000011486518],"about_ca_topic_score_codex":0.028799808,"about_ca_topic_score_gemma":0.01356717,"teacher_disagreement_score":0.028799808,"about_ca_system_score_codex":0.000618152,"about_ca_system_score_gemma":0.0002432718,"threshold_uncertainty_score":0.057264328},"labels":[],"label_agreement":null},{"id":"W2555530152","doi":"10.3847/1538-4357/834/1/15","title":"TYPE IA SUPERNOVAE: COLORS, RATES, AND PROGENITORS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"Supernova; Physics; Astrophysics; Galaxy; Star formation; Luminosity; Stars; Degenerate energy levels; Cutoff; Astronomy","score_opus":0.010874159417818397,"score_gpt":0.24474167152725457,"score_spread":0.23386751210943618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2555530152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963856,0.00039818336,0.0008542741,0.00002569861,0.0000025379031,0.000005108125,0.0006319691,0.000030632007,0.0016659419],"genre_scores_gemma":[0.99902916,0.00014095825,0.0002578802,0.0000054066822,0.0000041100893,0.0000018567152,0.00039385387,0.000005992973,0.00016081579],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977046,0.000050552084,0.000027451004,0.000068862646,0.00005268655,0.000030086645],"domain_scores_gemma":[0.99705243,0.0010954654,0.0009618956,0.00028361607,0.00031305212,0.0002934487],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011126476,0.0002204556,0.00018009718,0.0016598657,0.00014578609,0.0012036964,0.00038701043,0.00029386775,0.0011799751],"category_scores_gemma":[0.004108544,0.00018094854,0.00022826451,0.00090051664,0.00029707208,0.0005822676,0.00049062935,0.0002085404,0.00035654128],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006313251,0.000006895729,0.99534553,0.0000058741816,0.000019407042,0.000033248478,0.000030088417,0.00076744927,0.0011230473,0.0002980376,0.000036741723,0.0022705412],"study_design_scores_gemma":[0.0000033966653,0.00003159605,0.99347246,0.000008623485,0.000016468011,0.00035069414,0.00011401474,0.0038997578,0.0010428497,0.0006644551,0.0003871268,0.000008550975],"about_ca_topic_score_codex":0.002389218,"about_ca_topic_score_gemma":0.0020440358,"teacher_disagreement_score":0.002389218,"about_ca_system_score_codex":0.00033038983,"about_ca_system_score_gemma":0.00012133554,"threshold_uncertainty_score":0.0058843493},"labels":[],"label_agreement":null},{"id":"W2555968095","doi":"10.3847/1538-4357/835/2/153","title":"Galaxy Environment in the 3D-HST Fields: Witnessing the Onset of Satellite Quenching at z ∼ 1–2","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Galaxy; Halo; Satellite galaxy; Redshift; Sky; Photometry (optics); Grism; Stellar mass","score_opus":0.010776071165289433,"score_gpt":0.2223758372136169,"score_spread":0.21159976604832748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2555968095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989272,0.000036941656,0.00019497906,0.00002234215,9.433175e-7,0.0000021124345,0.0004912529,0.000027080425,0.00029715901],"genre_scores_gemma":[0.99889815,0.000011433034,0.0001505002,0.0000105122435,0.0000032393814,0.0000016553079,0.00083823234,0.000005660162,0.00008057231],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998729,0.000011854745,0.0000047721505,0.00003538107,0.00003465652,0.00004040702],"domain_scores_gemma":[0.9985971,0.00021488326,0.0005088341,0.00016207792,0.00019392805,0.0003232453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045279472,0.000116004034,0.00015252017,0.00082160666,0.00023233544,0.00039110667,0.00024923868,0.00020311978,0.0007976054],"category_scores_gemma":[0.0017725072,0.00012223402,0.00017663749,0.00055673084,0.00032714425,0.0003507215,0.0004954554,0.00024169992,0.00019086356],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012205263,0.000022530361,0.9887085,0.00000984716,0.000020094834,0.00010776705,0.00020140951,0.0014587572,0.0050738323,0.00028399852,0.0003546114,0.003636521],"study_design_scores_gemma":[0.0000014792778,0.0000081685885,0.9980501,0.0000013392817,0.0000031418977,0.00002328535,0.000028752389,0.0011804544,0.0004714245,0.000049911992,0.00017999779,0.000001962032],"about_ca_topic_score_codex":0.013213275,"about_ca_topic_score_gemma":0.014722857,"teacher_disagreement_score":0.013213275,"about_ca_system_score_codex":0.0005246503,"about_ca_system_score_gemma":0.00016585493,"threshold_uncertainty_score":0.026272714},"labels":[],"label_agreement":null},{"id":"W2556952860","doi":"10.3847/0004-637x/831/2/192","title":"MULTI-WAVELENGTH STUDY OF THE SUPERNOVA REMNANT KES 79 (G33.6+0.1): ON ITS SUPERNOVA PROPERTIES AND EXPANSION INTO A MOLECULAR ENVIRONMENT","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Supernova; Astrophysics; Halo; Ionization; Plasma; Supernova remnant; Molecular cloud; Atomic physics; Galaxy; Ion; Stars; Nuclear physics","score_opus":0.022684690080136446,"score_gpt":0.2159247949502602,"score_spread":0.19324010487012377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2556952860","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99944323,0.0000783414,0.000055630404,0.000006323159,0.0000011867536,0.0000018551798,0.00009543876,0.0000056232097,0.00031233596],"genre_scores_gemma":[0.9992944,0.000043422744,0.00016813206,0.00001060748,0.000003929614,0.0000018840063,0.0002321599,0.0000069876733,0.0002384589],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.0000021449619,0.0000015763735,0.000011820965,0.000007242409,0.000009126991],"domain_scores_gemma":[0.99989974,0.000008396459,0.000031271575,0.000007663816,0.000016227981,0.000036691545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008635583,0.00018435708,0.00015820796,0.000508095,0.00025403503,0.00022503754,0.00016821221,0.00017238557,0.0005320416],"category_scores_gemma":[0.000074980744,0.000106291845,0.00019384683,0.00032832375,0.00013480187,0.00014044985,0.00025569712,0.00019405452,0.00023423004],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003411786,0.00011960857,0.4267298,0.000043815657,0.0000854764,0.0020437164,0.0002574504,0.00047859197,0.5633495,0.0001551496,0.0002535568,0.0061422046],"study_design_scores_gemma":[0.00000297559,0.00006519229,0.99386865,0.0000020409839,0.00001618267,0.0006336008,0.00010394734,0.00033399832,0.0045209755,0.000020095706,0.00042839837,0.0000039899105],"about_ca_topic_score_codex":0.0018097466,"about_ca_topic_score_gemma":0.002805388,"teacher_disagreement_score":0.0018097466,"about_ca_system_score_codex":0.00016066404,"about_ca_system_score_gemma":0.000059641665,"threshold_uncertainty_score":0.0035985112},"labels":[],"label_agreement":null},{"id":"W2557533654","doi":"10.3847/1538-4357/ab63dd","title":"Investigating Overdensities around z &gt; 6 Galaxies through ALMA Observations of [C ii]","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Dalhousie University","funders":"","keywords":"Physics; Astrophysics; Reionization; Galaxy; QSOS; Luminosity; Context (archaeology); Luminosity function; Hubble Deep Field; Astronomy; Universe; Luminous infrared galaxy; Quasar; Redshift","score_opus":0.029083978195687837,"score_gpt":0.22823748624386092,"score_spread":0.19915350804817308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2557533654","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952555,0.00001706469,0.00011570969,0.0000067733736,5.042122e-7,0.0000011050523,0.00006904164,0.000009332807,0.00025489746],"genre_scores_gemma":[0.9997373,0.000006686072,0.000101961654,0.0000027395342,0.0000013111614,5.4242236e-7,0.0000844996,8.8278756e-7,0.00006401576],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999062,0.000011597005,0.0000043635337,0.000027593536,0.000024988876,0.00002518667],"domain_scores_gemma":[0.999292,0.00011362641,0.0003136991,0.00006660338,0.00008025531,0.00013381928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020252896,0.00010957,0.000108237764,0.001062059,0.00026607854,0.00059731543,0.00020290723,0.00014747423,0.0009576662],"category_scores_gemma":[0.0007975188,0.000101230275,0.000118141026,0.00060027174,0.00020342735,0.00029576418,0.00034350774,0.00012388195,0.00014359206],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050415732,0.00001750068,0.9869474,0.00000458256,0.00002338431,0.000075718715,0.0001912603,0.00028907688,0.008903478,0.00011603644,0.00009416852,0.0032869813],"study_design_scores_gemma":[8.9306326e-7,0.000010959506,0.9987644,8.2534297e-7,0.0000052883315,0.000036689224,0.00004425544,0.00050654094,0.000474742,0.00002813841,0.00012608212,0.0000012272725],"about_ca_topic_score_codex":0.007564701,"about_ca_topic_score_gemma":0.01191742,"teacher_disagreement_score":0.007564701,"about_ca_system_score_codex":0.00030146303,"about_ca_system_score_gemma":0.000085760126,"threshold_uncertainty_score":0.015041351},"labels":[],"label_agreement":null},{"id":"W2558123270","doi":"10.3847/1538-4357/aa6b5a","title":"The Proper Motion of Pyxis: The First Use of Adaptive Optics in Tandem with HST on a Faint Halo Object","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Proper motion; Halo; Milky Way; Adaptive optics; Globular cluster; Galactic halo; Motion (physics); Astrometry","score_opus":0.016818469458480086,"score_gpt":0.21374497797578343,"score_spread":0.19692650851730334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2558123270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982951,0.000053843443,0.0008183738,0.000018135484,0.000003135888,0.000005683333,0.00021212491,0.000032073145,0.0005615316],"genre_scores_gemma":[0.9978399,0.00003115853,0.0016378949,0.000006282517,0.0000058762007,0.0000032305502,0.00030921173,0.0000072847897,0.00015913106],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985003,0.000019338013,0.000006766338,0.00004154969,0.000059230384,0.000023006],"domain_scores_gemma":[0.9995183,0.000045637757,0.000121275945,0.000113204296,0.00009787724,0.00010382615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042550193,0.00022992503,0.00017729489,0.0011258562,0.0003764855,0.00037683666,0.00027363712,0.00014534485,0.00048318718],"category_scores_gemma":[0.0006475794,0.00016168602,0.0002468221,0.00078404107,0.000367365,0.00025504388,0.0006357881,0.0002016011,0.00017676216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032955882,0.00004014113,0.88986796,0.000053658296,0.00013439062,0.00069611747,0.00044980165,0.00348622,0.08296193,0.00039466654,0.00040921895,0.021176325],"study_design_scores_gemma":[0.000009193475,0.00008486935,0.98591983,0.000006512253,0.000027102293,0.00024142285,0.000106933025,0.005969452,0.006867758,0.00011010063,0.0006446943,0.000012144211],"about_ca_topic_score_codex":0.0044900896,"about_ca_topic_score_gemma":0.006310162,"teacher_disagreement_score":0.0044900896,"about_ca_system_score_codex":0.00036331048,"about_ca_system_score_gemma":0.00032248293,"threshold_uncertainty_score":0.008927882},"labels":[],"label_agreement":null},{"id":"W2558440077","doi":"10.3847/1538-4357/aa72d8","title":"The Rest-frame Optical (900 nm) Galaxy Luminosity Function at z ∼ 4–7: Abundance Matching Points to Limited Evolution in the M<sub>STAR</sub>/M<sub>HALO</sub> Ratio at z ≥ 4","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy; Luminosity; Luminosity function; Mass-to-light ratio; Stars; Stellar population; Line (geometry); Optical depth; Stellar evolution","score_opus":0.009076230033858707,"score_gpt":0.21651602420759247,"score_spread":0.20743979417373376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2558440077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996406,0.000036747846,0.00045463536,0.00001898003,0.0000018024364,0.0000017903176,0.0010908503,0.00007946919,0.001909816],"genre_scores_gemma":[0.99751365,0.000015060545,0.0003987718,0.000010273103,0.0000025647341,0.0000017982007,0.0016364758,0.00001094668,0.0004105446],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994457,0.0000030034125,0.0000016902028,0.00001431425,0.000010344155,0.000026024378],"domain_scores_gemma":[0.9997316,0.000029990482,0.00008290863,0.000021904312,0.00006373767,0.000069731155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014741742,0.000150728,0.00010405822,0.0011236956,0.00014859499,0.00046917525,0.000233937,0.00016969968,0.0024268897],"category_scores_gemma":[0.00025905276,0.000080313155,0.00018896368,0.00041616728,0.00013630383,0.00021457612,0.00021489042,0.00015744015,0.00095167616],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014620676,0.000026696074,0.9603658,0.000012843312,0.000036276513,0.00008587064,0.000082931954,0.0005235074,0.025316432,0.00031581623,0.00086163334,0.0122260675],"study_design_scores_gemma":[7.65977e-7,0.0000069075145,0.9972759,0.0000017864307,0.000006906869,0.00002781807,0.00004819917,0.0008032766,0.0014957273,0.000038837563,0.000292633,0.0000013630843],"about_ca_topic_score_codex":0.0082769785,"about_ca_topic_score_gemma":0.011460668,"teacher_disagreement_score":0.0082769785,"about_ca_system_score_codex":0.00027409982,"about_ca_system_score_gemma":0.00010363983,"threshold_uncertainty_score":0.016457558},"labels":[],"label_agreement":null},{"id":"W2558762085","doi":"10.3847/1538-4357/834/2/163","title":"SWIFT OBSERVATIONS OF TWO OUTBURSTS FROM THE MAGNETAR 4U 0142+61","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University; McGill University Health Centre","funders":"","keywords":"Magnetar; Glitch; Pulsar; Physics; Swift; Astrophysics; Event (particle physics); Neutron star; Telescope; Astronomy","score_opus":0.036311693234853074,"score_gpt":0.34528253144191534,"score_spread":0.3089708382070623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2558762085","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992466,0.000026018071,0.000056602174,0.000017258226,0.0000065758018,0.000005588848,0.00009091641,0.0000067494334,0.0005437572],"genre_scores_gemma":[0.99884135,0.000030324814,0.00022679048,0.000033872166,0.00001978391,0.00001220225,0.00050992396,0.000004956791,0.00032091778],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998647,0.000013951626,0.000008517876,0.00003042112,0.00003990925,0.000042504857],"domain_scores_gemma":[0.9995363,0.000047997473,0.00012565815,0.000043943888,0.000067496934,0.00017867427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030237058,0.00025943638,0.00037376303,0.00094046077,0.00086777145,0.00055834104,0.00021718838,0.00045648732,0.00056326046],"category_scores_gemma":[0.00060140126,0.00021645427,0.000176363,0.00056930335,0.00028808604,0.00020090837,0.0010246655,0.00042275264,0.0001434511],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005292949,0.00026486447,0.89013,0.00005608092,0.0000995547,0.0034496065,0.0015079014,0.000530225,0.08596367,0.00038277128,0.0009862273,0.016099842],"study_design_scores_gemma":[0.000011312775,0.00011214708,0.99748933,0.0000050640447,0.000010326129,0.0003547137,0.0001555877,0.00020355085,0.0007205584,0.000034770317,0.0008967241,0.000005895986],"about_ca_topic_score_codex":0.0037201939,"about_ca_topic_score_gemma":0.010111289,"teacher_disagreement_score":0.0037201939,"about_ca_system_score_codex":0.00022545717,"about_ca_system_score_gemma":0.00020304426,"threshold_uncertainty_score":0.0073970556},"labels":[],"label_agreement":null},{"id":"W2559266421","doi":"10.3847/1538-4357/aa830c","title":"An Upper Limit on the Mass of a Central Black Hole in the Large Magellanic Cloud from the Stellar Rotation Field","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Supermassive black hole; Black hole (networking); Astronomy; Galactic Center; Large Magellanic Cloud; Very Large Telescope; Telescope; Galactic plane","score_opus":0.010293221634748235,"score_gpt":0.22650767540252284,"score_spread":0.2162144537677746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2559266421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9772389,0.0024993783,0.0119756,0.00022459317,0.00003659162,0.000009991028,0.00050487026,0.00015545145,0.00735462],"genre_scores_gemma":[0.99828184,0.0001568398,0.0011494607,0.000028340535,0.000039999508,0.0000023926732,0.00020405381,0.000007443534,0.00012963326],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983144,0.000025430481,0.0000061921664,0.00005012358,0.000043183318,0.000043654905],"domain_scores_gemma":[0.9983381,0.00068559585,0.00038686255,0.00017658023,0.00015915616,0.00025367917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078260904,0.0004378164,0.00030853626,0.0010524562,0.00041429224,0.0008829722,0.0005341274,0.00046172927,0.0026168944],"category_scores_gemma":[0.0023153762,0.00014187339,0.00028768586,0.00029660255,0.00058169814,0.00059281336,0.00072076765,0.00031069372,0.00047047425],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045891284,0.00007465286,0.8502145,0.00017916986,0.00015353473,0.0005121901,0.00026563334,0.0076386225,0.08394075,0.019308422,0.0014093769,0.03584415],"study_design_scores_gemma":[0.00003093823,0.00012747807,0.9218992,0.00013944122,0.00010776015,0.00051698193,0.0002127805,0.036454096,0.015655372,0.018430324,0.006386439,0.000039223887],"about_ca_topic_score_codex":0.0021270066,"about_ca_topic_score_gemma":0.002518277,"teacher_disagreement_score":0.0026168944,"about_ca_system_score_codex":0.00037927442,"about_ca_system_score_gemma":0.00012660792,"threshold_uncertainty_score":0.008754373},"labels":[],"label_agreement":null},{"id":"W2559346263","doi":"10.3847/1538-4357/835/2/217","title":"Millimeter-wave Line Ratios and Sub-beam Volume Density Distributions","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Isotopologue; Line (geometry); Log-normal distribution; Range (aeronautics); Power law; Volume (thermodynamics); Probability density function; Electron density","score_opus":0.01206845646557263,"score_gpt":0.2186034786393122,"score_spread":0.20653502217373956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2559346263","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8637962,0.0004125875,0.11873566,0.00042057305,0.000021396032,0.000032621912,0.003139263,0.001245872,0.012195809],"genre_scores_gemma":[0.9931164,0.0000640451,0.005400746,0.00003533198,0.000009228632,0.000010260663,0.00064593664,0.0000922766,0.0006256357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997166,0.00008784844,0.000013886962,0.000082943756,0.00005952695,0.000039243805],"domain_scores_gemma":[0.99642843,0.0020935328,0.00062563247,0.000454918,0.0002935838,0.00010384402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007766482,0.0002266549,0.00017018286,0.0010217144,0.00014048346,0.0007055498,0.000588822,0.00029824977,0.0029645676],"category_scores_gemma":[0.0050010458,0.00013431585,0.00021237199,0.0008225713,0.00029452608,0.0013845712,0.00036679913,0.00031006432,0.0004744948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027527387,0.000082590515,0.6577172,0.00010946266,0.00017482726,0.00032421702,0.00037504532,0.20922607,0.0264914,0.03191252,0.0031610928,0.0701503],"study_design_scores_gemma":[0.000021654334,0.00006149374,0.3240368,0.000027253665,0.000042626107,0.00028000897,0.00024510457,0.6297389,0.023185644,0.018214617,0.0041003707,0.00004552445],"about_ca_topic_score_codex":0.004330587,"about_ca_topic_score_gemma":0.002238624,"teacher_disagreement_score":0.004330587,"about_ca_system_score_codex":0.0004532423,"about_ca_system_score_gemma":0.000070073016,"threshold_uncertainty_score":0.009917438},"labels":[],"label_agreement":null},{"id":"W2560169568","doi":"10.3847/1538-4357/aa60c1","title":"Energetics and Birth Rates of Supernova Remnants in the Large Magellanic Cloud","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Large Magellanic Cloud; Supernova; Energy distribution; Dispersion (optics); Energy density; Energetics; Shock wave; Computational astrophysics; Stellar evolution","score_opus":0.01314025218565984,"score_gpt":0.25334521078102745,"score_spread":0.2402049585953676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2560169568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994885,0.00009238758,0.000067153036,0.0000028807794,3.7040576e-7,0.0000013731919,0.00019020752,0.000007303794,0.00014994256],"genre_scores_gemma":[0.99908364,0.000058583555,0.00006353062,0.000001177757,9.2833966e-7,0.000001165811,0.0006796985,0.00000408554,0.000107205946],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998956,0.000016508495,0.00001090162,0.000027855047,0.000022200398,0.000026988562],"domain_scores_gemma":[0.99932754,0.00026649339,0.0001977921,0.00006441002,0.00006932933,0.00007451043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005537487,0.00016139215,0.00013144728,0.0012824769,0.0001551005,0.00046223024,0.00028316324,0.00016140199,0.00092297257],"category_scores_gemma":[0.0014887098,0.00010416604,0.00034578666,0.00046532726,0.00016195745,0.0001943369,0.00022703818,0.00008461942,0.00020725334],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020896849,0.000025269095,0.983055,0.000022399137,0.000096798474,0.00025007318,0.00008531989,0.0068692067,0.005050591,0.00031931206,0.00011539642,0.0039016076],"study_design_scores_gemma":[0.000007143626,0.000050325358,0.99001175,0.0000059562813,0.000028949074,0.0002463324,0.00009415053,0.0074423603,0.0017562254,0.00010352085,0.00024694376,0.00000634015],"about_ca_topic_score_codex":0.006802208,"about_ca_topic_score_gemma":0.0051998976,"teacher_disagreement_score":0.006802208,"about_ca_system_score_codex":0.0004419755,"about_ca_system_score_gemma":0.00012726165,"threshold_uncertainty_score":0.013525188},"labels":[],"label_agreement":null},{"id":"W2561327819","doi":"10.3847/1538-4357/aa5ebb","title":"Gravitational Waves from F-modes Excited by the Inspiral of Highly Eccentric Neutron Star Binaries","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Neutron star; Gravitational wave; Einstein Telescope; Amplitude; General relativity; Numerical relativity; Excited state; Neutron; Gravitational redshift","score_opus":0.014827325722836066,"score_gpt":0.3025389811657213,"score_spread":0.28771165544288524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2561327819","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950629,0.000072460105,0.0020299135,0.00008182369,0.000011861117,0.000005405232,0.00007083127,0.00004204105,0.00262273],"genre_scores_gemma":[0.9985354,0.000031271793,0.0008158314,0.000023457209,0.0000075389457,0.0000023628395,0.00009579869,0.000014840583,0.00047357287],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999399,0.000010913984,0.000002933148,0.000010257218,0.000020367072,0.00001549729],"domain_scores_gemma":[0.9995116,0.00014182733,0.00010094664,0.000050579496,0.000057300746,0.00013781094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003871905,0.00023043025,0.00029167495,0.00038778578,0.00051831926,0.00062886043,0.00031387337,0.00030212163,0.0014981434],"category_scores_gemma":[0.0010330279,0.00017541443,0.0002831441,0.00029596756,0.0003119626,0.00039776653,0.0007775801,0.000575325,0.00018196138],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023026569,0.00053354644,0.483305,0.0002616522,0.00068239425,0.003620011,0.0020824214,0.13096483,0.2802195,0.039835297,0.003257822,0.052934833],"study_design_scores_gemma":[0.00012005821,0.000517557,0.5360148,0.000058607257,0.00009212612,0.00068574754,0.00069415715,0.41558138,0.022998316,0.019399278,0.003710945,0.00012699858],"about_ca_topic_score_codex":0.0022897904,"about_ca_topic_score_gemma":0.0023886508,"teacher_disagreement_score":0.0022897904,"about_ca_system_score_codex":0.0004511349,"about_ca_system_score_gemma":0.00016203083,"threshold_uncertainty_score":0.0050117373},"labels":[],"label_agreement":null},{"id":"W2561412421","doi":"10.3847/1538-4357/834/1/66","title":"THE NEXT GENERATION VIRGO CLUSTER SURVEY. XXII. SHELL FEATURE EARLY-TYPE DWARF GALAXIES IN THE VIRGO CLUSTER*","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Physics; Virgo Cluster; Astrophysics; Surface brightness; Astronomy; Galaxy; Galaxy cluster; Dwarf galaxy; RADIUS; Cluster (spacecraft)","score_opus":0.02466824793835728,"score_gpt":0.24606326908308715,"score_spread":0.22139502114472986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2561412421","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9768819,0.00035972946,0.00034403426,0.00007673653,0.000007597808,0.00003718739,0.01922645,0.00006669904,0.0029997258],"genre_scores_gemma":[0.97743326,0.000116698495,0.000711427,0.000024463692,0.000006985122,0.000024047235,0.020617142,0.000013310219,0.0010526024],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989974,0.000017224622,0.000005679595,0.000024533476,0.0000274655,0.000025304915],"domain_scores_gemma":[0.9997805,0.00002967186,0.00005287922,0.00003111756,0.000037361162,0.000068469046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002669254,0.0001400771,0.00015270906,0.001105136,0.0002465105,0.00034009718,0.00024935685,0.00018608873,0.0016520458],"category_scores_gemma":[0.0004156271,0.000076054814,0.00017306014,0.000908617,0.00010081105,0.00014183282,0.0003585072,0.00009877863,0.0005275802],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008174262,0.00003759857,0.9843226,0.000034395354,0.000047046735,0.00006792669,0.000091918046,0.0016018697,0.0017347502,0.0003832398,0.0034173059,0.008179744],"study_design_scores_gemma":[0.000005853253,0.000009883871,0.99605054,0.0000037631469,0.000009132982,0.000033826713,0.00004878304,0.0016275854,0.00024578348,0.00005610761,0.0019054459,0.0000033936367],"about_ca_topic_score_codex":0.033543672,"about_ca_topic_score_gemma":0.045707244,"teacher_disagreement_score":0.033543672,"about_ca_system_score_codex":0.00047013105,"about_ca_system_score_gemma":0.00017885957,"threshold_uncertainty_score":0.06669688},"labels":[],"label_agreement":null},{"id":"W2562102770","doi":"10.3847/1538-4357/835/2/292","title":"Non-LTE Stellar Population Synthesis of Globular Clusters Using Synthetic Integrated Light Spectra. I. Constructing the IL Spectra","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Globular cluster; Spectral line; Stellar population; Population; Stars; Hertzsprung–Russell diagram; Astronomical spectroscopy; Stellar evolution; Horizontal branch","score_opus":0.01252449906987037,"score_gpt":0.23413941610401945,"score_spread":0.22161491703414907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2562102770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93198854,0.00002233076,0.065511085,0.000021485546,0.000007409029,0.00004947497,0.0005442665,0.0005141014,0.001341213],"genre_scores_gemma":[0.96244204,0.000013032441,0.0361339,0.000013082624,0.0000039729603,0.000043244094,0.000977386,0.000120862394,0.00025238073],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998677,0.000038158676,0.00000739043,0.000037924492,0.000031203126,0.000017616909],"domain_scores_gemma":[0.9991917,0.00034498447,0.00007352456,0.0001526159,0.00019240312,0.00004478644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005657869,0.0003201142,0.00019519356,0.00048353348,0.0002740264,0.00043463733,0.0005630189,0.00021563277,0.0008558118],"category_scores_gemma":[0.002380752,0.00023170917,0.00041732754,0.00036752806,0.00019257239,0.00023333622,0.00037428844,0.00024588962,0.00021145951],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029881706,0.00009814233,0.078132994,0.00006257737,0.00009025383,0.00015089136,0.00031839474,0.85135996,0.026715182,0.003778924,0.0004557468,0.038538124],"study_design_scores_gemma":[0.000034734614,0.00004281849,0.017891003,0.000003978105,0.0000121445455,0.000024531977,0.00005415511,0.9701505,0.010021539,0.0011696311,0.00058169005,0.0000132350815],"about_ca_topic_score_codex":0.0072568255,"about_ca_topic_score_gemma":0.0057176086,"teacher_disagreement_score":0.0072568255,"about_ca_system_score_codex":0.00077628,"about_ca_system_score_gemma":0.0003959519,"threshold_uncertainty_score":0.014429212},"labels":[],"label_agreement":null},{"id":"W2562358469","doi":"10.3847/1538-4357/835/1/101","title":"GLOBULAR CLUSTER SYSTEMS IN BRIGHTEST CLUSTER GALAXIES. III. BEYOND BIMODALITY","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Bimodality; Galaxy cluster; Brightest cluster galaxy; Galaxy; Coma Cluster; Metallicity; Dwarf galaxy","score_opus":0.008590370315995513,"score_gpt":0.22635135548509044,"score_spread":0.21776098516909492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2562358469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99785775,0.00033752917,0.00018712078,0.00004440377,0.0000031046475,0.0000025926997,0.00028072426,0.000028942817,0.0012577813],"genre_scores_gemma":[0.99958235,0.000023446135,0.000068563415,0.000011558606,0.0000032104344,0.0000010406308,0.00017026393,0.0000026337086,0.00013693713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998111,0.000012214749,0.000009069417,0.00006433042,0.00003079574,0.00007250032],"domain_scores_gemma":[0.9988661,0.00011307757,0.00040225784,0.00012843059,0.00014184714,0.00034841642],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023353743,0.00017262717,0.0002794666,0.002027886,0.00043598952,0.0008542166,0.00030203897,0.00029025518,0.0030744548],"category_scores_gemma":[0.00086371443,0.00014655295,0.00016087973,0.0010447457,0.00066966057,0.00054585485,0.0010459761,0.0003015435,0.0004608479],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016719796,0.000020175974,0.97782487,0.00002558231,0.000023881543,0.00016037293,0.00045260316,0.00022061357,0.012747068,0.00079693185,0.00025476416,0.007305926],"study_design_scores_gemma":[0.000002998735,0.000011587275,0.9981207,0.000004031935,0.000005564325,0.00014059093,0.00013017027,0.00025060438,0.0004330481,0.00048500497,0.00041291796,0.0000027798378],"about_ca_topic_score_codex":0.007528723,"about_ca_topic_score_gemma":0.00928225,"teacher_disagreement_score":0.007528723,"about_ca_system_score_codex":0.0006028024,"about_ca_system_score_gemma":0.00021592493,"threshold_uncertainty_score":0.014969826},"labels":[],"label_agreement":null},{"id":"W2562468229","doi":"10.3847/1538-4357/833/2/199","title":"SPECTRAL EVOLUTION IN HIGH REDSHIFT QUASARS FROM THE FINAL BARYON OSCILLATION SPECTROSCOPIC SURVEY SAMPLE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Notre Dame; Leibniz-Gemeinschaft; University of Colorado Boulder; High Energy Physics; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; York University; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Johns Hopkins University; University of Washington; Carnegie Institution of Washington; University of Utah; Ohio State University; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik; U.S. Department of Energy; Smithsonian Institution","keywords":"Astrophysics; Physics; Redshift; Quasar; Luminosity; Population; Spectral index; Spectral line; Astronomy; Galaxy","score_opus":0.01372644107485676,"score_gpt":0.2246348025103544,"score_spread":0.21090836143549763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2562468229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995301,0.00002304351,0.00008446162,0.0000055374303,0.0000014689726,0.0000012787534,0.00023740588,0.000004406563,0.00011239238],"genre_scores_gemma":[0.99823844,0.00002418512,0.00016583595,0.0000068575628,0.000004905527,0.0000034356337,0.0014345754,0.0000060438183,0.00011570096],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967706,0.00005038959,0.000021849854,0.00006920756,0.000104253835,0.00007728176],"domain_scores_gemma":[0.998585,0.00022133053,0.0005126955,0.0001523482,0.0002617686,0.00026683506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000660416,0.00019391208,0.00021678866,0.0016230126,0.00028759317,0.0006124965,0.0001886301,0.00017865536,0.0006651116],"category_scores_gemma":[0.0016998216,0.00013225872,0.00018440332,0.00077710085,0.0002030758,0.00020950401,0.00073702465,0.00017454317,0.00024625257],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006909128,0.0000148292065,0.9904518,0.0000045944785,0.000028882752,0.000054871285,0.00013807697,0.00006952944,0.0062457826,0.000037001082,0.000098567514,0.0027870669],"study_design_scores_gemma":[9.718915e-7,0.000011716281,0.99947685,6.749698e-7,0.000004270076,0.00006260741,0.00003817939,0.00008670843,0.00018668354,0.000008221968,0.0001219987,0.0000012217661],"about_ca_topic_score_codex":0.0029444136,"about_ca_topic_score_gemma":0.004733174,"teacher_disagreement_score":0.0029444136,"about_ca_system_score_codex":0.0001368307,"about_ca_system_score_gemma":0.000092966504,"threshold_uncertainty_score":0},"labels":[],"label_agreement":null},{"id":"W2562824716","doi":"10.3847/1538-4357/aa73df","title":"The NANOGrav Nine-year Data Set: Measurement and Analysis of Variations in Dispersion Measures","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; California Institute of Technology; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Universities Space Research Association; West Virginia University; National Science Foundation","keywords":"Pulsar; Millisecond pulsar; Physics; Astrophysics; Dispersion (optics); Function (biology); Statistical physics; Biology; Optics","score_opus":0.05600580191034149,"score_gpt":0.3559215803852776,"score_spread":0.2999157784749361,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2562824716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9501466,0.0001716751,0.0010172189,0.0001138117,0.00003278965,0.000030829684,0.046273574,0.00012339438,0.002090133],"genre_scores_gemma":[0.88660115,0.000095531126,0.0022285809,0.0000404242,0.000037609203,0.000083578074,0.11015287,0.000045122262,0.0007151325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99899834,0.0001554514,0.00013743184,0.0002088879,0.0004272552,0.000072614646],"domain_scores_gemma":[0.9940593,0.0013216547,0.0018351815,0.0012938598,0.0011699527,0.00031997098],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014758988,0.00024803396,0.0003341623,0.003470077,0.00034912146,0.0006301597,0.00050073094,0.00029417864,0.00076785556],"category_scores_gemma":[0.004497628,0.0001253013,0.00023512774,0.0036586504,0.00019443939,0.0005822262,0.0008922142,0.00029902134,0.0004715453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001911405,0.00005558157,0.97622615,0.00004522751,0.00012490776,0.00009856529,0.00017984504,0.001705243,0.001922139,0.0002729483,0.0050168876,0.014161332],"study_design_scores_gemma":[0.000010630702,0.000028381673,0.9905716,0.000008494599,0.000015875114,0.00007168278,0.0001239002,0.0032048835,0.0007241282,0.00009187773,0.005135343,0.000013226663],"about_ca_topic_score_codex":0.0137306545,"about_ca_topic_score_gemma":0.020811452,"teacher_disagreement_score":0.0137306545,"about_ca_system_score_codex":0.00044688027,"about_ca_system_score_gemma":0.0003082405,"threshold_uncertainty_score":0.02730143},"labels":[],"label_agreement":null},{"id":"W2562876616","doi":"10.3847/1538-4357/aa5b91","title":"Detection of Time Lags between Quasar Continuum Emission Bands Based On Pan-STARRS Light Curves","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Smithsonian Astrophysical Observatory; Eötvös Loránd Tudományegyetem; National Central University; Queen's University Belfast; Office of Science; Max-Planck-Institut für Astronomie; University of Edinburgh; Durham University; York University; Space Telescope Science Institute; Carnegie Mellon University; University of Arizona; Los Alamos National Laboratory; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Harvard University; Queen's University; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University","keywords":"Light curve; Quasar; Gravitational microlensing; Redshift; Accretion disc; Accretion (finance); Emission spectrum; Rest frame; Line (geometry)","score_opus":0.007696954117537249,"score_gpt":0.22218073687120576,"score_spread":0.21448378275366853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2562876616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988018,0.000091287664,0.00026695538,0.000006685379,0.000003299371,0.000002097002,0.00043702024,0.000020831936,0.00037007508],"genre_scores_gemma":[0.9991571,0.000020496804,0.00015918528,0.0000027014823,0.0000061640303,0.0000024604667,0.00057428074,0.0000033618917,0.00007416031],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981123,0.00002260947,0.000017103868,0.00006228848,0.00004127435,0.0000455241],"domain_scores_gemma":[0.9973393,0.0006005385,0.0012589423,0.0001386185,0.00025267727,0.00040994567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046772402,0.0002003341,0.00016791592,0.0019201301,0.00015384395,0.00044773967,0.00017565761,0.00021632634,0.0011355636],"category_scores_gemma":[0.0014933314,0.00011854468,0.00019203148,0.0008055292,0.00016719074,0.000332992,0.00038348767,0.00019215529,0.00024874182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012685823,0.00002156992,0.9866897,0.0000191079,0.00003538669,0.00009409393,0.00009919711,0.00023366312,0.0077412287,0.000076728924,0.000105980675,0.0047564195],"study_design_scores_gemma":[0.0000012315319,0.000024194425,0.99913687,0.0000018278181,0.000004542119,0.000054022992,0.000029641113,0.00020384292,0.0003436782,0.000014813794,0.0001835884,0.0000018410437],"about_ca_topic_score_codex":0.0012742686,"about_ca_topic_score_gemma":0.0018610097,"teacher_disagreement_score":0.0019201301,"about_ca_system_score_codex":0.00015833322,"about_ca_system_score_gemma":0.00007987643,"threshold_uncertainty_score":0.0037988424},"labels":[],"label_agreement":null},{"id":"W2564108058","doi":"10.3847/1538-4357/aa6d5c","title":"Shock Dynamics in Stellar Outbursts. I. Shock Formation","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Supernova; Shock wave; Shock (circulatory); Dissipation; Astrophysics; Radiative transfer; Shock waves in astrophysics; Moving shock; Luminosity; Mechanics; Optics","score_opus":0.012789088345338864,"score_gpt":0.243391754266953,"score_spread":0.23060266592161413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2564108058","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950793,0.00011692124,0.0037743016,0.00002706274,0.0000045539773,0.000008197847,0.00004504205,0.000022540393,0.0009221299],"genre_scores_gemma":[0.9992291,0.000066242246,0.00032247472,0.0000034292834,0.0000020275559,0.0000028515674,0.000045938166,0.000004126793,0.00032391227],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999511,0.000010584167,0.000005268675,0.00001080398,0.000010196347,0.000011960594],"domain_scores_gemma":[0.99956363,0.000092563416,0.00019039641,0.000028479786,0.000040757845,0.00008419496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021640267,0.00025802266,0.00021771021,0.0003452004,0.00022665902,0.0005091383,0.00022759475,0.00029075844,0.0008752417],"category_scores_gemma":[0.0010145269,0.00014968302,0.00025183568,0.00022184452,0.0004325892,0.00033275143,0.00059778924,0.0002907906,0.00010389265],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076240033,0.00017918467,0.3295677,0.00018441706,0.00013568708,0.0027149403,0.0014026815,0.48608685,0.12627967,0.031651452,0.00063236017,0.020402614],"study_design_scores_gemma":[0.000041179574,0.00031459637,0.13024057,0.00002683235,0.000034234527,0.0006534142,0.0005119881,0.8483446,0.009655971,0.009256923,0.00089003,0.00002971654],"about_ca_topic_score_codex":0.0017131739,"about_ca_topic_score_gemma":0.00062225986,"teacher_disagreement_score":0.0017131739,"about_ca_system_score_codex":0.0003429776,"about_ca_system_score_gemma":0.00011377511,"threshold_uncertainty_score":0.0034063458},"labels":[],"label_agreement":null},{"id":"W2564331575","doi":"10.3847/1538-4357/834/1/40","title":"ULTRAVIOLET ESCAPE FRACTIONS FROM GIANT MOLECULAR CLOUDS DURING EARLY CLUSTER FORMATION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Molecular cloud; Star formation; Cluster (spacecraft); Radiative transfer; Ionization; Photon; Flux (metallurgy); Protostar; Interstellar medium","score_opus":0.0060799328516498,"score_gpt":0.2166934851822785,"score_spread":0.2106135523306287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2564331575","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943453,0.000016190419,0.00021569939,0.000011456718,0.0000011701753,0.0000015944328,0.000048493104,0.00001348134,0.00025729663],"genre_scores_gemma":[0.99978775,0.000007914618,0.00006937641,0.0000024957303,7.023049e-7,0.0000015158562,0.00007930042,0.000003951228,0.00004711164],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994993,0.000006130361,0.0000022207926,0.00000853436,0.0000091835345,0.000023979483],"domain_scores_gemma":[0.9997291,0.000109988854,0.000050777468,0.000017947104,0.000026881715,0.000065197564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021581007,0.00029099445,0.00018592733,0.00027009958,0.00033159336,0.00048550952,0.0002847258,0.00028734625,0.0005204761],"category_scores_gemma":[0.00080580445,0.00015908488,0.0003912137,0.00021911903,0.00030254995,0.00022896205,0.0003332114,0.00028371534,0.000050172515],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000577985,0.00014110944,0.35787657,0.00008826125,0.00016657321,0.00084685924,0.00023439244,0.563239,0.06906866,0.0024107918,0.00041656668,0.0049333237],"study_design_scores_gemma":[0.00009254227,0.00025042664,0.35147497,0.000015210851,0.000063635045,0.00026847137,0.00014756275,0.63345873,0.01282554,0.0009579084,0.00041330807,0.000031689742],"about_ca_topic_score_codex":0.0069500944,"about_ca_topic_score_gemma":0.0043125027,"teacher_disagreement_score":0.0069500944,"about_ca_system_score_codex":0.0006735082,"about_ca_system_score_gemma":0.00027061198,"threshold_uncertainty_score":0.013819277},"labels":[],"label_agreement":null},{"id":"W2565610924","doi":"10.3847/1538-4357/835/2/210","title":"Polarization Gradient Study of Interstellar Medium Turbulence Using the Canadian Galactic Plane Survey","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; National Research Council Canada; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Polarization (electrochemistry); Interstellar medium; Turbulence; Galaxy; Skewness; Kurtosis; Chemistry; Statistics; Meteorology","score_opus":0.03138030383985297,"score_gpt":0.27174353464493295,"score_spread":0.24036323080507999,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2565610924","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99471056,0.00007454827,0.00025044533,0.000049768943,0.000003055237,0.000012803047,0.0031213507,0.000014925088,0.0017625702],"genre_scores_gemma":[0.9954372,0.00007641844,0.0004568546,0.000014233209,0.000002931768,0.000005705984,0.0035146144,0.0000061243486,0.0004858065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99964535,0.00002980454,0.000007780193,0.000058080685,0.0001448969,0.00011409678],"domain_scores_gemma":[0.99910766,0.00005338522,0.00011259373,0.000049979364,0.0005192645,0.00015715467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003129698,0.0002817645,0.00016482576,0.0022463717,0.00083475455,0.0007056409,0.00036556946,0.00014465587,0.00075555895],"category_scores_gemma":[0.00090426404,0.0001295079,0.00020408792,0.003463068,0.0003305092,0.00023524211,0.00047289545,0.0002479245,0.00013858789],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000098211734,0.000017275723,0.98581475,0.0000144896985,0.00005801094,0.00008878065,0.0003405924,0.0011909035,0.0035256778,0.00031144422,0.0012753963,0.007264568],"study_design_scores_gemma":[0.0000022211898,0.0000052055516,0.9977138,0.000002981399,0.000006531896,0.000018963463,0.00017595156,0.00080378493,0.00030221118,0.000012417604,0.0009495863,0.000006361816],"about_ca_topic_score_codex":0.9519313,"about_ca_topic_score_gemma":0.9684641,"teacher_disagreement_score":0.9519313,"about_ca_system_score_codex":0.004139661,"about_ca_system_score_gemma":0.0035115718,"threshold_uncertainty_score":0.09670353},"labels":[],"label_agreement":null},{"id":"W2565963586","doi":"10.3847/1538-4357/835/1/45","title":"THE CONTRIBUTION OF FERMI-2LAC BLAZARS TO DIFFUSE TEV–PEV NEUTRINO FLUX","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":267,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Blazar; Physics; Neutrino; Astrophysics; Fermi Gamma-ray Space Telescope; Flux (metallurgy); Spectral index; Neutrino detector; Astronomy; Neutrino astronomy; Cosmic ray; Neutrino oscillation; Particle physics; Spectral line; Gamma ray","score_opus":0.008454698440240625,"score_gpt":0.24150293861045458,"score_spread":0.23304824017021394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2565963586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99520004,0.00018806459,0.0015735001,0.000049216844,0.0000030875208,0.0000050446947,0.0008366859,0.00008456968,0.0020597975],"genre_scores_gemma":[0.9978035,0.00003457902,0.00043596205,0.000014278738,0.000007027989,0.000004100766,0.0013014032,0.000012196456,0.00038697282],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996755,0.000066427754,0.000014095173,0.00010757453,0.00006285517,0.00007365015],"domain_scores_gemma":[0.9986745,0.0005288998,0.00035615062,0.00018368186,0.00012162579,0.00013507695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007401617,0.00038833867,0.00030664538,0.0014932809,0.0003438983,0.0013683107,0.000264501,0.00034883965,0.0032943333],"category_scores_gemma":[0.0022162083,0.00021152283,0.00047737625,0.0006256707,0.00024390398,0.00033542237,0.0005750593,0.0002374636,0.00041060834],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037896924,0.000024813704,0.9745619,0.000035499746,0.00014547346,0.0001533382,0.000094548246,0.0030635167,0.008799793,0.0007551214,0.00048034295,0.01150656],"study_design_scores_gemma":[0.000015279216,0.000045002394,0.98400176,0.000015536356,0.00006868717,0.0002874428,0.00010277061,0.011235207,0.0024973021,0.0006027726,0.0011140202,0.000014274621],"about_ca_topic_score_codex":0.003673296,"about_ca_topic_score_gemma":0.003941657,"teacher_disagreement_score":0.003673296,"about_ca_system_score_codex":0.00037036964,"about_ca_system_score_gemma":0.00017956906,"threshold_uncertainty_score":0.011020601},"labels":[],"label_agreement":null},{"id":"W2566374048","doi":"10.3847/1538-4357/833/2/127","title":"A SPECTROSCOPIC SEARCH FOR CHEMICALLY STRATIFIED WHITE DWARFS IN THE SLOAN DIGITAL SKY SURVEY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Natural Sciences and Engineering Research Council of Canada; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"White dwarf; Physics; Sky; Astrophysics; Helium; Astronomy; Stars; Stellar classification; Spectral line","score_opus":0.0197619492275283,"score_gpt":0.2545523808848038,"score_spread":0.2347904316572755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2566374048","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978668,0.00008588598,0.0003094478,0.000018172832,0.0000011442505,0.000012414098,0.0011290194,0.00003370539,0.00054337154],"genre_scores_gemma":[0.9951573,0.00007676291,0.000755124,0.000025054145,0.0000034010081,0.000010112995,0.0034888738,0.0000103331195,0.0004729634],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977344,0.000022159107,0.000017062364,0.000050687693,0.00007838634,0.000058259],"domain_scores_gemma":[0.9993724,0.0000452823,0.00019440927,0.000070600996,0.000096137475,0.000221177],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040330697,0.00022949556,0.00017054772,0.0018353226,0.0004897266,0.00048007135,0.00017904605,0.0001118015,0.0008128637],"category_scores_gemma":[0.000444645,0.00012779317,0.00018758322,0.001724336,0.00020795605,0.0001804241,0.00061002985,0.00008980445,0.00029056196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006185449,0.000022599887,0.98471284,0.000019984733,0.000048914688,0.00009580311,0.0002613045,0.00029335075,0.008392198,0.00016466648,0.0006544345,0.005272105],"study_design_scores_gemma":[0.0000036829042,0.000015934982,0.9969049,0.0000027194621,0.000012839897,0.00004150497,0.00015473853,0.0006305086,0.0009128882,0.000036038586,0.0012815308,0.0000026182884],"about_ca_topic_score_codex":0.023884827,"about_ca_topic_score_gemma":0.055282965,"teacher_disagreement_score":0.023884827,"about_ca_system_score_codex":0.00048601307,"about_ca_system_score_gemma":0.0005420036,"threshold_uncertainty_score":0.04749161},"labels":[],"label_agreement":null},{"id":"W2567172099","doi":"10.3847/1538-4357/835/2/184","title":"The Relation Between Globular Cluster Systems and Supermassive Black Holes in Spiral Galaxies: The Case Study of NGC 4258","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Globular cluster; Supermassive black hole; Spiral galaxy; Milky Way; Galaxy; Star cluster; Photometry (optics); Intermediate-mass black hole; Black hole (networking)","score_opus":0.01440045743345579,"score_gpt":0.24478497424047344,"score_spread":0.23038451680701766,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2567172099","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942267,0.000064570166,0.000029741857,0.00003580918,4.7369787e-7,0.0000020825044,0.00004251732,0.0000019215986,0.0004002088],"genre_scores_gemma":[0.9997701,0.000029009792,0.00003256276,0.000004054385,0.0000020384512,0.00000110274,0.00004602234,7.326005e-7,0.00011439889],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997259,0.000080489255,0.00001967987,0.000044421613,0.000050858478,0.00007866747],"domain_scores_gemma":[0.9987907,0.0004470778,0.00026426208,0.000094110954,0.0001140002,0.00029002817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042722744,0.00027143786,0.00024094591,0.0018278246,0.0008135054,0.00090429286,0.00038375994,0.0003770111,0.0015946705],"category_scores_gemma":[0.0015676252,0.000113223796,0.00021660971,0.0015881382,0.00077130424,0.0003065121,0.0006773478,0.00022572647,0.00014134786],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046286514,0.000028439843,0.9957943,0.000007962429,0.000019683534,0.001540724,0.0004637619,0.00021526082,0.00029133592,0.0002390194,0.00011549122,0.0012376753],"study_design_scores_gemma":[0.0000106640055,0.00006891201,0.99225557,0.000010290646,0.000046985482,0.00239774,0.0027591805,0.0013508842,0.00018421702,0.00034477405,0.00056096073,0.000009887032],"about_ca_topic_score_codex":0.06277323,"about_ca_topic_score_gemma":0.06854259,"teacher_disagreement_score":0.06277323,"about_ca_system_score_codex":0.00071190647,"about_ca_system_score_gemma":0.0003197128,"threshold_uncertainty_score":0.1248157},"labels":[],"label_agreement":null},{"id":"W2567230118","doi":"10.3847/1538-4357/835/2/141","title":"Preconditioning of Interplanetary Space Due to Transient CME Disturbances","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Natural Resources Canada","funders":"","keywords":"Coronal mass ejection; Solar wind; Interplanetary spaceflight; Physics; Space weather; Interplanetary space; Solar cycle 23; Astrophysics; Atmospheric sciences; Astronomy; Plasma","score_opus":0.006617259936410225,"score_gpt":0.23334179515228115,"score_spread":0.22672453521587094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2567230118","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99705374,0.00008533213,0.0019126658,0.000018732973,0.000010741839,0.000005219356,0.00025797015,0.000061435705,0.00059428526],"genre_scores_gemma":[0.9995542,0.0000177386,0.00014681372,0.0000030999647,0.00000480966,0.0000016229608,0.00022379565,0.0000068060863,0.000041056603],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998216,0.000015220867,0.000012603857,0.00006222602,0.000043323842,0.0000450985],"domain_scores_gemma":[0.999206,0.00020763403,0.00024927565,0.000108911576,0.000089177185,0.00013890152],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002090991,0.00021643384,0.00027261922,0.00038129665,0.00016561993,0.00045728975,0.00026522548,0.00026386476,0.0011560649],"category_scores_gemma":[0.0013797665,0.000099156605,0.00031841852,0.0003247735,0.00025060764,0.0003556676,0.00059028354,0.0003383602,0.00010400208],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015111913,0.0002475797,0.6561005,0.00028902094,0.0004817797,0.002066493,0.00045210027,0.18244489,0.10756404,0.0015028574,0.0012992417,0.046040285],"study_design_scores_gemma":[0.000020743222,0.00020214733,0.9065628,0.000016576341,0.000053566113,0.00024380391,0.00013096712,0.0855701,0.0059313015,0.00039628003,0.00084927055,0.000022434291],"about_ca_topic_score_codex":0.0030293697,"about_ca_topic_score_gemma":0.0014757793,"teacher_disagreement_score":0.0030293697,"about_ca_system_score_codex":0.00026662377,"about_ca_system_score_gemma":0.00018072646,"threshold_uncertainty_score":0.0060234666},"labels":[],"label_agreement":null},{"id":"W2567237302","doi":"10.3847/1538-4357/835/2/123","title":"Globular Clusters as Tracers of Fine Structure in the Dramatic Shell Galaxy NGC 474","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Globular cluster; Galaxy; Halo; Accretion (finance); Population; Elliptical galaxy; Galaxy merger; Dust lane; Stars","score_opus":0.0066251686075606,"score_gpt":0.22467663631062107,"score_spread":0.21805146770306047,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2567237302","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990466,0.00004984256,0.00018821118,0.000007788699,0.0000010584224,0.0000022101171,0.0001102083,0.000016618633,0.0005773711],"genre_scores_gemma":[0.9994733,0.000019028128,0.00021068295,0.000004352229,0.0000018725202,0.000001698315,0.0001760233,0.000003436847,0.00010955698],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998746,0.000022217555,0.000005470482,0.000031560023,0.000032693184,0.000033477834],"domain_scores_gemma":[0.99908864,0.00019707123,0.00028594313,0.00009736224,0.000114268696,0.00021676926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002254071,0.00011550865,0.00016296249,0.0019040736,0.00033707987,0.0005353007,0.00021441557,0.00020637132,0.000815129],"category_scores_gemma":[0.0007567378,0.00012871921,0.00011374204,0.0011755286,0.00046016747,0.0002312651,0.0007526668,0.0001943658,0.00013265379],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000112915746,0.000016620374,0.9725161,0.000011010222,0.000048353126,0.00009905467,0.00024272299,0.0011237974,0.022008017,0.00059377594,0.00019633636,0.0030311828],"study_design_scores_gemma":[0.000003907568,0.000020954345,0.996612,0.0000027221604,0.000009173458,0.00005750492,0.00015917399,0.001425143,0.0011186037,0.00025655533,0.00032959387,0.0000045773063],"about_ca_topic_score_codex":0.013352308,"about_ca_topic_score_gemma":0.011919014,"teacher_disagreement_score":0.013352308,"about_ca_system_score_codex":0.0005553743,"about_ca_system_score_gemma":0.00015537196,"threshold_uncertainty_score":0.02654916},"labels":[],"label_agreement":null},{"id":"W2567283754","doi":"10.3847/1538-4357/835/1/61","title":"CHROMOSPHERICALLY ACTIVE STARS IN THE RAVE SURVEY. II. YOUNG DWARFS IN THE SOLAR NEIGHBORHOOD","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leibniz-Gemeinschaft; Natural Sciences and Engineering Research Council of Canada; Deutsche Forschungsgemeinschaft; Javna Agencija za Raziskovalno Dejavnost RS; Macquarie University; W. M. Keck Foundation; Agence Nationale de la Recherche; National Aeronautics and Space Administration; California Institute of Technology; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Johns Hopkins University; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Stars; Starspot; Hertzsprung–Russell diagram; Main sequence; T Tauri star; Diagram; Flux (metallurgy); Infrared; K-type main-sequence star","score_opus":0.016334959697567875,"score_gpt":0.24674737772699795,"score_spread":0.23041241802943008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2567283754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981686,0.0003572118,0.000100931626,0.0000089260075,0.000001921086,0.000004077841,0.00066125515,0.000008453377,0.0006887201],"genre_scores_gemma":[0.9973712,0.00021098401,0.00016819364,0.000007759976,0.000005308839,0.000003094782,0.0016450535,0.000003818052,0.0005844593],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997403,0.000038726015,0.000026826776,0.00009872196,0.000053172207,0.00004222159],"domain_scores_gemma":[0.9995735,0.00005895295,0.000118695476,0.0000658191,0.00007381745,0.0001093133],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038507432,0.00010351815,0.000272348,0.0018571226,0.00018060535,0.00041817134,0.00012548879,0.00014303355,0.0009827192],"category_scores_gemma":[0.00058192026,0.000083095314,0.00017954578,0.0007058376,0.000109130175,0.00031695561,0.00055771205,0.00009536079,0.0005747218],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051809046,0.000015532712,0.9878191,0.000019093122,0.000024355837,0.000068464156,0.00020138574,0.00005950516,0.002864445,0.000052782543,0.000115344854,0.008708107],"study_design_scores_gemma":[7.499909e-7,0.000024483435,0.9986981,0.0000026303528,0.0000052575583,0.0001687185,0.0001309505,0.000049472903,0.0001776103,0.000008584518,0.0007325287,8.57943e-7],"about_ca_topic_score_codex":0.0014164371,"about_ca_topic_score_gemma":0.0029955734,"teacher_disagreement_score":0.0018571226,"about_ca_system_score_codex":0.00007548984,"about_ca_system_score_gemma":0.0000701305,"threshold_uncertainty_score":0.0032875538},"labels":[],"label_agreement":null},{"id":"W2567350882","doi":"10.3847/1538-4357/aa6d64","title":"The Galaxy–Halo Connection in High-redshift Universe: Details and Evolution of Stellar-to-halo Mass Ratios of Lyman Break Galaxies on CFHTLS Deep Fields","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Halo; Galaxy; Stellar mass; Satellite galaxy; Satellite; Telescope; Mass distribution; Spectral energy distribution; Mass ratio","score_opus":0.006341990618677642,"score_gpt":0.20849275941564985,"score_spread":0.20215076879697222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2567350882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962926,0.000014009104,0.000094901654,0.000004378843,2.2785996e-7,7.294836e-7,0.00012120685,0.000008782824,0.00012647912],"genre_scores_gemma":[0.9996038,0.000005190573,0.00010781967,0.0000013659482,6.5527723e-7,6.42029e-7,0.00023226767,0.0000020665625,0.000046214478],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998735,0.000023457842,0.0000051554616,0.00003729824,0.000026265698,0.000034416207],"domain_scores_gemma":[0.9989636,0.0003261112,0.00025004102,0.0001111128,0.0001416243,0.00020746849],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046886856,0.00016484305,0.000111957146,0.0013810075,0.00022550492,0.00048062537,0.00021027368,0.00021029434,0.00085324363],"category_scores_gemma":[0.0014878474,0.00012052362,0.00023233966,0.0005843248,0.00028248885,0.00026650913,0.0003519603,0.00013723395,0.00012347462],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060090424,0.00001308498,0.98979646,0.0000048492116,0.000035880876,0.000032535747,0.00010336764,0.004110861,0.0032481216,0.00021406203,0.00010016146,0.002280632],"study_design_scores_gemma":[0.0000013630168,0.000005935306,0.994719,9.53314e-7,0.0000042487363,0.0000104247765,0.000032693973,0.0048386995,0.0002954901,0.000033274515,0.000055439094,0.0000023897885],"about_ca_topic_score_codex":0.02606607,"about_ca_topic_score_gemma":0.02093993,"teacher_disagreement_score":0.02606607,"about_ca_system_score_codex":0.00052074034,"about_ca_system_score_gemma":0.00016226181,"threshold_uncertainty_score":0.051828682},"labels":[],"label_agreement":null},{"id":"W2567564655","doi":"10.3847/1538-4357/834/2/104","title":"THE 2015 DECAY OF THE BLACK HOLE X-RAY BINARY V404 CYGNI: ROBUST DISK-JET COUPLING AND A SHARP TRANSITION INTO QUIESCENCE","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Luminosity; Black hole (networking); Accretion (finance); Jansky; Galaxy; Radio galaxy","score_opus":0.016346544565282548,"score_gpt":0.24810709920656762,"score_spread":0.2317605546412851,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2567564655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991781,0.000034127395,0.000080698264,0.000030905954,0.0000035071214,0.00000260843,0.00007663126,0.000007454644,0.0005859689],"genre_scores_gemma":[0.9994999,0.000015218379,0.00005199548,0.000012700137,0.000005608683,0.0000019956346,0.00019341892,0.0000030095844,0.0002161107],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999161,0.0000069851294,0.000004332486,0.000023308492,0.000023208897,0.000026081454],"domain_scores_gemma":[0.9997067,0.000019527835,0.00010236012,0.000024516507,0.000046820547,0.00010007195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022888152,0.00018178242,0.00020891793,0.00046426945,0.00046678222,0.00059466437,0.00017238474,0.00022504847,0.00089252414],"category_scores_gemma":[0.00058937306,0.00011083311,0.00011399883,0.00022455913,0.0003539668,0.00022014136,0.00084605324,0.00030036597,0.00015884676],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038557273,0.00009344298,0.9259847,0.000034393524,0.000054142878,0.0010710559,0.0011569383,0.00040829513,0.060541783,0.0009521916,0.00062358053,0.008693893],"study_design_scores_gemma":[0.000002898645,0.00006890621,0.99741924,0.0000056274876,0.000007028633,0.00013174585,0.00018394974,0.0002414757,0.001207705,0.00009837364,0.00062906794,0.000003869095],"about_ca_topic_score_codex":0.004804923,"about_ca_topic_score_gemma":0.0070118587,"teacher_disagreement_score":0.004804923,"about_ca_system_score_codex":0.00049661833,"about_ca_system_score_gemma":0.00020742176,"threshold_uncertainty_score":0.009553909},"labels":[],"label_agreement":null},{"id":"W2569283353","doi":"10.3847/0004-637x/817/2/136","title":"SIMULATIONS OF ENERGETIC PARTICLES INTERACTING WITH DYNAMICAL MAGNETIC TURBULENCE","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Turbulence; Test particle; K-epsilon turbulence model; Solar wind; K-omega turbulence model; Magnetic field; Statistical physics; Classical mechanics; Magnetohydrodynamics; Computational physics; Mechanics","score_opus":0.005201665836941475,"score_gpt":0.21622581634741317,"score_spread":0.2110241505104717,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2569283353","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99477684,0.000041913045,0.0025122252,0.00009499126,0.000018104967,0.000015255452,0.00010524094,0.0000450825,0.0023903414],"genre_scores_gemma":[0.9984982,0.000020237796,0.0010113707,0.000017437305,0.0000048230663,0.000014613038,0.00011197256,0.000010447103,0.000310908],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998134,0.00005504826,0.000010442593,0.000023636974,0.000039491726,0.000058080033],"domain_scores_gemma":[0.99827325,0.0010511035,0.00016018673,0.000111359564,0.00017423528,0.00022991712],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039919885,0.00043528274,0.0006813672,0.00059171964,0.00071484636,0.0008814134,0.0011764028,0.0012956174,0.0018070362],"category_scores_gemma":[0.0022322393,0.00028995622,0.0005413396,0.0006745247,0.0009241284,0.0006999726,0.00066231703,0.00079066155,0.0001274568],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018043802,0.000169609,0.005434151,0.000020456924,0.00006104178,0.00020137073,0.00007100911,0.9888104,0.0015535183,0.0023704271,0.00014637464,0.0009811082],"study_design_scores_gemma":[0.00004306963,0.000047764388,0.00073477573,0.0000027071803,0.000006570526,0.000009625388,0.000027144875,0.9981974,0.00048559668,0.00034346146,0.00009623052,0.000005670969],"about_ca_topic_score_codex":0.013861653,"about_ca_topic_score_gemma":0.005214456,"teacher_disagreement_score":0.013861653,"about_ca_system_score_codex":0.00081197964,"about_ca_system_score_gemma":0.0006045195,"threshold_uncertainty_score":0.027561963},"labels":[],"label_agreement":null},{"id":"W2569502108","doi":"10.3847/1538-4357/835/2/264","title":"Hubble Space Telescope Detection of the Millisecond Pulsar J2124−3358 and its Far-ultraviolet Bow Shock Nebula","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Pulsar; Nebula; Millisecond pulsar; Astronomy; Neutron star; Bow shock (aerodynamics); RADIUS; Pulsar wind nebula; Telescope; Stars; Shock wave","score_opus":0.01143815198559625,"score_gpt":0.2915179797346158,"score_spread":0.28007982774901957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2569502108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873465,0.00007342327,0.00012934448,0.00002792345,0.0000044014855,0.0000034005693,0.000102927675,0.000022872304,0.0009009783],"genre_scores_gemma":[0.9990231,0.000020610478,0.0002313347,0.000014413057,0.0000065465647,0.0000026126304,0.00018920591,0.0000017023585,0.0005105411],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999232,0.000008375215,0.0000034208826,0.000016834385,0.000026480442,0.000021599562],"domain_scores_gemma":[0.99982315,0.000009749642,0.00005427686,0.0000119071,0.000021795518,0.00007913166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015207854,0.00023435337,0.0001534251,0.00062885834,0.00047143246,0.0003174074,0.00023043575,0.00030055532,0.0018367453],"category_scores_gemma":[0.00032376507,0.0001323796,0.00013833202,0.00028326127,0.00011121148,0.00011614672,0.00031912207,0.00017095346,0.00028118162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006988188,0.00011349219,0.7708081,0.000052366395,0.00012546769,0.0011931479,0.0004582083,0.00047962126,0.19824737,0.00060853787,0.00099061,0.026224252],"study_design_scores_gemma":[0.000019480703,0.00015312272,0.99234617,0.0000069104394,0.000027320477,0.00047116523,0.000090209134,0.0006921639,0.003981053,0.00008035596,0.002124029,0.000007938695],"about_ca_topic_score_codex":0.0050282967,"about_ca_topic_score_gemma":0.010579793,"teacher_disagreement_score":0.0050282967,"about_ca_system_score_codex":0.0003380645,"about_ca_system_score_gemma":0.00010593768,"threshold_uncertainty_score":0.009998083},"labels":[],"label_agreement":null},{"id":"W2572195087","doi":"10.3847/1538-4357/836/1/123","title":"CO-Dark Star Formation and Black Hole Activity in 3C 368 at z = 1.131: Coeval Growth of Stellar and Supermassive Black Hole Masses<sup>∗</sup> <sup>†</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Supermassive black hole; Star formation; Neon; Galaxy; Active galactic nucleus; Astronomy; Metallicity","score_opus":0.010523047756700701,"score_gpt":0.23007887339378583,"score_spread":0.21955582563708512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2572195087","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999532,0.000014308302,0.000018540119,0.000018189552,0.0000011754561,0.0000012580089,0.0001893205,0.0000037719162,0.00022148591],"genre_scores_gemma":[0.99965084,0.000007211466,0.000030468496,0.00000554221,0.0000020516075,8.812241e-7,0.00021050245,0.0000014638356,0.00009110364],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994135,0.000004195893,0.0000038647663,0.000014560626,0.000016189208,0.000019905396],"domain_scores_gemma":[0.99963784,0.00002829067,0.00014657906,0.000019389045,0.00004278397,0.0001250793],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000100085854,0.00016714835,0.00017403961,0.0005463291,0.00029569567,0.00037542768,0.00024162597,0.00032233447,0.0017804862],"category_scores_gemma":[0.00031954856,0.00007845143,0.00012609272,0.00033032117,0.00025862115,0.00015460819,0.00026674708,0.0002038934,0.00042365835],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000112790454,0.000030520827,0.98836225,0.0000062060785,0.000013116672,0.00022646584,0.00013962072,0.000099564466,0.0094248215,0.00004707131,0.00013783114,0.0013996729],"study_design_scores_gemma":[0.0000011615374,0.000011262199,0.9992924,7.2863577e-7,0.000003815798,0.00008378768,0.00007034682,0.00010814522,0.00031018376,0.000014382871,0.00010216872,0.000001426684],"about_ca_topic_score_codex":0.014902086,"about_ca_topic_score_gemma":0.024645189,"teacher_disagreement_score":0.014902086,"about_ca_system_score_codex":0.00031597508,"about_ca_system_score_gemma":0.00009361895,"threshold_uncertainty_score":0.029630661},"labels":[],"label_agreement":null},{"id":"W2572432525","doi":"10.3847/1538-4357/835/2/255","title":"Rate Constants for Fine-structure Excitations in O–H Collisions with Error Bars Obtained by Machine Learning","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Forecasting Techniques and Applications","field":"Decision Sciences","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Adiabatic process; Sensitivity (control systems); Reaction rate constant; Gaussian; Physics; Computation; Ab initio; Adiabatic theorem; Atomic physics; Scattering; Inelastic scattering; Quantum mechanics; Algorithm; Computer science","score_opus":0.0670230049671471,"score_gpt":0.37300124272455665,"score_spread":0.30597823775740957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2572432525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8180455,0.00026809628,0.17780486,0.00030108602,0.00005050936,0.00003412918,0.00023979775,0.000623719,0.0026323537],"genre_scores_gemma":[0.9882658,0.00003411266,0.011166651,0.000023020973,0.000008786828,0.00001602923,0.00012159051,0.00004775696,0.0003162329],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99938774,0.00021246161,0.00003331983,0.00010048301,0.00018668719,0.00007928109],"domain_scores_gemma":[0.99107504,0.0067238854,0.00075750845,0.0007555885,0.0005607097,0.00012718895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0040406385,0.00045028576,0.00050641724,0.0009273377,0.000616215,0.0006488783,0.0014889842,0.0007201696,0.001081299],"category_scores_gemma":[0.010762411,0.00027686468,0.00064632925,0.00081319106,0.0008295212,0.00090794277,0.00061025255,0.0010554323,0.00013831962],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009143244,0.00005318498,0.0038769916,0.000017695229,0.000033348904,0.000027496493,0.000027034132,0.9833793,0.0018239281,0.0059617152,0.00013424159,0.0045736786],"study_design_scores_gemma":[0.0000031496468,0.0000044838657,0.0006337406,0.0000019666818,0.0000029863543,0.0000040354807,0.0000024851827,0.99661297,0.0014690958,0.0012351847,0.00002378559,0.0000061365195],"about_ca_topic_score_codex":0.008566228,"about_ca_topic_score_gemma":0.004309549,"teacher_disagreement_score":0.008566228,"about_ca_system_score_codex":0.0011132138,"about_ca_system_score_gemma":0.0010685994,"threshold_uncertainty_score":0.021369219},"labels":[],"label_agreement":null},{"id":"W2573673530","doi":"10.3847/1538-4357/836/2/174","title":"Extragalactic Peaked-spectrum Radio Sources at Low Frequencies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":167,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Spectral index; Galaxy; Spectral line; Redshift; Source counts; Radio spectrum; Sample (material); Synchrotron; Radio galaxy","score_opus":0.009160198052195248,"score_gpt":0.21199164921700386,"score_spread":0.2028314511648086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2573673530","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998437,0.00007782904,0.00020243012,0.000011797509,0.0000010627098,0.0000072854446,0.0006502658,0.000015859576,0.0005965183],"genre_scores_gemma":[0.9979067,0.0000561111,0.00022352353,0.000015300677,0.000005884822,0.000008860252,0.0015173509,0.000006139237,0.00026031065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984884,0.000023289815,0.0000106202515,0.000031693635,0.00004031798,0.000045234723],"domain_scores_gemma":[0.99919003,0.00013155464,0.00034388795,0.00009854311,0.00009344398,0.00014243017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018824721,0.00020871268,0.00023574104,0.0017187226,0.00024265955,0.00047602577,0.00023879088,0.00012915925,0.0029713658],"category_scores_gemma":[0.0007304926,0.00011636921,0.00015935164,0.0011470345,0.00018625578,0.00024330961,0.0004976305,0.00013644776,0.0007703383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000915427,0.000022642726,0.98870146,0.0000122617175,0.000022733731,0.0001317099,0.00014560601,0.00006726474,0.0052086865,0.000083608444,0.00029153452,0.0052209203],"study_design_scores_gemma":[0.0000031633417,0.000012268358,0.99867415,0.0000029472458,0.000008347874,0.00021712903,0.00007409337,0.000102923404,0.0004962534,0.000033314045,0.00037382654,0.0000016592921],"about_ca_topic_score_codex":0.0016967391,"about_ca_topic_score_gemma":0.0029182702,"teacher_disagreement_score":0.0029713658,"about_ca_system_score_codex":0.0001207378,"about_ca_system_score_gemma":0.000073368166,"threshold_uncertainty_score":0.009940147},"labels":[],"label_agreement":null},{"id":"W2575579273","doi":"10.3847/1538-4357/aa82bb","title":"CMB Polarization B-mode Delensing with SPTpol and Herschel","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; Canadian Institute for Advanced Research","funders":"Argonne National Laboratory; Natural Sciences and Engineering Research Council of Canada; University of Colorado Boulder; Office of Science; Canada Research Chairs; McGill University; Gordon and Betty Moore Foundation; U.S. Department of Energy; University of Chicago; Croucher Foundation; National Science Foundation","keywords":"Cosmic microwave background; Multipole expansion; Physics; Gravitational lens; Gravitational wave; Polarization (electrochemistry); Sky; Astrophysics; Anisotropy; Noise (video); Spectral density; Mode (computer interface); Computational physics; Optics; Galaxy; Quantum mechanics; Computer science; Telecommunications","score_opus":0.007288559882366625,"score_gpt":0.25464019099435337,"score_spread":0.24735163111198674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2575579273","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9757829,0.000053267337,0.01451878,0.00021501364,0.000026114305,0.000021927792,0.0015946954,0.0012141425,0.00657323],"genre_scores_gemma":[0.98718876,0.000019893196,0.010520144,0.000041842828,0.000008730633,0.000015453437,0.0015879219,0.00016937849,0.0004478674],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99945015,0.00018543312,0.000012856655,0.00010659726,0.0001660515,0.00007890098],"domain_scores_gemma":[0.99868697,0.0005127434,0.00016258498,0.00037533243,0.00015376248,0.000108544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011543004,0.00034657677,0.00029047526,0.00038256787,0.0003807135,0.00071709056,0.0007697227,0.00036413572,0.0025894234],"category_scores_gemma":[0.0032421998,0.00028093296,0.00047321516,0.0005414286,0.00043310935,0.0005646892,0.0008558872,0.0007094033,0.00035377906],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008235262,0.00014614021,0.11074846,0.00010876543,0.00035645813,0.0005598415,0.0002853267,0.82171756,0.02077065,0.012580155,0.0037433007,0.028159847],"study_design_scores_gemma":[0.0001466426,0.000098422184,0.06386399,0.0000185509,0.000042656964,0.00014020051,0.00008306764,0.9063335,0.01945952,0.0055236625,0.0042092903,0.000080571444],"about_ca_topic_score_codex":0.013380784,"about_ca_topic_score_gemma":0.013738683,"teacher_disagreement_score":0.013380784,"about_ca_system_score_codex":0.00084066746,"about_ca_system_score_gemma":0.00044797684,"threshold_uncertainty_score":0.026605844},"labels":[],"label_agreement":null},{"id":"W2577513478","doi":"10.1088/0004-637x/815/1/56","title":"A NEW ANALYSIS OF THE TWO CLASSICAL ZZ CETI WHITE DWARFS GD 165 AND ROSS 548. I. PHOTOMETRY AND SPECTROSCOPY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Langara College; Université de Montréal","funders":"","keywords":"Physics; White dwarf; Multiplet; Photometry (optics); Stars; Astrophysics; Spectroscopy; Light curve; Astronomy; Spectral line","score_opus":0.013497651339475707,"score_gpt":0.2558206336977898,"score_spread":0.2423229823583141,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2577513478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911097,0.00017252532,0.0049830745,0.00004218084,0.000011020344,0.000021728767,0.00065592706,0.00006460138,0.0029391802],"genre_scores_gemma":[0.9862673,0.00008336753,0.009605126,0.000024980605,0.000019521098,0.000012631613,0.0025479938,0.000028911953,0.0014101061],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998004,0.000014463998,0.000016853039,0.00008029806,0.00006283288,0.000025269288],"domain_scores_gemma":[0.9997303,0.000024831197,0.000073160016,0.00005192079,0.000060391885,0.000059331887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021616551,0.00032573257,0.00023810202,0.0015453574,0.00029322968,0.0005023427,0.00024009947,0.00017367475,0.0009922212],"category_scores_gemma":[0.0004455774,0.00011971302,0.00032805276,0.0007196022,0.00018483655,0.00028144018,0.0006993835,0.00016220396,0.00024883577],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035991316,0.00009724864,0.48014432,0.00012885343,0.00018940984,0.00092244765,0.00050216314,0.0021906416,0.43894246,0.0019233823,0.00079184864,0.07380734],"study_design_scores_gemma":[0.000014807378,0.00012828578,0.97179633,0.0000084750445,0.0000747184,0.00079480157,0.00023290844,0.008795826,0.011701838,0.0006537756,0.0057802564,0.000018028064],"about_ca_topic_score_codex":0.0041685477,"about_ca_topic_score_gemma":0.011667491,"teacher_disagreement_score":0.0041685477,"about_ca_system_score_codex":0.00033193146,"about_ca_system_score_gemma":0.00019665385,"threshold_uncertainty_score":0.008288562},"labels":[],"label_agreement":null},{"id":"W2579155888","doi":"10.3847/1538-4357/835/2/288","title":"Search for Magnetically Broadened Cascade Emission from Blazars with VERITAS","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Blazar; Astrophysics; Cascade; Cosmic microwave background; Gamma ray; Photon; Intergalactic travel; Active galactic nucleus; Compton scattering; Electron; Positron; Galaxy; Redshift; Nuclear physics; Optics","score_opus":0.012348616693885855,"score_gpt":0.25131040867874954,"score_spread":0.2389617919848637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2579155888","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967533,0.00013837028,0.0011213393,0.000032631648,0.0000046249443,0.000015486563,0.0003456751,0.00008452664,0.0015041052],"genre_scores_gemma":[0.9967218,0.00004582941,0.0015939889,0.000024056226,0.0000135078,0.000008263061,0.001251982,0.000013614729,0.0003269683],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996376,0.000033232653,0.000014079244,0.00011180683,0.00011041134,0.00009280992],"domain_scores_gemma":[0.9984621,0.0003274483,0.00074127485,0.0001220975,0.00010634432,0.00024077244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006086418,0.00064541603,0.00036326525,0.0014610041,0.0004932193,0.0007522151,0.0006629703,0.00051088113,0.002814154],"category_scores_gemma":[0.00092750695,0.00035167942,0.0004116683,0.0006909671,0.00027878373,0.000324876,0.0007067261,0.0004298095,0.00036300873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009903888,0.00016611938,0.8751107,0.00012648174,0.00027778695,0.0014957689,0.00035448314,0.004131195,0.099885926,0.001310945,0.00077462575,0.015375624],"study_design_scores_gemma":[0.00012377957,0.0004618565,0.965208,0.000042194,0.0002353143,0.0011315896,0.00021764905,0.01452309,0.014358854,0.000497847,0.0031687766,0.00003108417],"about_ca_topic_score_codex":0.0036627564,"about_ca_topic_score_gemma":0.007919469,"teacher_disagreement_score":0.0036627564,"about_ca_system_score_codex":0.00045098102,"about_ca_system_score_gemma":0.0003218404,"threshold_uncertainty_score":0.009414256},"labels":[],"label_agreement":null},{"id":"W2580852603","doi":"10.3847/1538-4357/aa677f","title":"First Search for Gravitational Waves from Known Pulsars with Advanced LIGO","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":195,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; National Research Foundation; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Istituto Nazionale di Fisica Nucleare; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Ministerio de Economía y Competitividad; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Govern de les Illes Balears; European Commission; Russian Foundation for Basic Research; Leverhulme Trust; Scottish Funding Council; Scottish Universities Physics Alliance; Hungarian Scientific Research Fund; Science and Technology Facilities Council; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Fundação de Amparo à Pesquisa do Estado de São Paulo; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; LIGO; Pulsar; Gravitational wave; Amplitude; Gravitational-wave observatory; Astrophysics; Astronomy; Limit (mathematics); Detector; Neutron star; Spin (aerodynamics); Optics","score_opus":0.01680221136847093,"score_gpt":0.32917696749302694,"score_spread":0.312374756124556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2580852603","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870372,0.0006811647,0.006704069,0.00026283634,0.000025305004,0.000025266905,0.0013063134,0.00022202975,0.003735879],"genre_scores_gemma":[0.99007684,0.00015597898,0.005947248,0.00022448832,0.000044960136,0.000020922686,0.00295309,0.000032511056,0.0005440334],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989003,0.00026349508,0.00006657461,0.00022037221,0.00034195188,0.00020729612],"domain_scores_gemma":[0.9954846,0.0022301238,0.0005887398,0.00084014714,0.00037386868,0.0004825707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018918378,0.00044468697,0.0005565218,0.0018927222,0.00055950746,0.001356378,0.00041218236,0.00069615204,0.0013232353],"category_scores_gemma":[0.0038481879,0.00043903425,0.00043006038,0.0011860111,0.0005478345,0.000845967,0.001530439,0.0008412664,0.0005782146],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013096975,0.00033535063,0.86493236,0.00016735085,0.0008482988,0.00074242055,0.00055650563,0.0015983107,0.06805214,0.0032046,0.0034075996,0.05484541],"study_design_scores_gemma":[0.0002020092,0.00086884364,0.9213136,0.000058747228,0.00056614185,0.0011408759,0.00022442095,0.009478426,0.04139082,0.00540787,0.019236328,0.00011192389],"about_ca_topic_score_codex":0.0006450726,"about_ca_topic_score_gemma":0.001467488,"teacher_disagreement_score":0.0018927222,"about_ca_system_score_codex":0.00027076117,"about_ca_system_score_gemma":0.00022880056,"threshold_uncertainty_score":0.010005116},"labels":[],"label_agreement":null},{"id":"W2580872109","doi":"10.3847/1538-4357/836/2/198","title":"The PAH Emission Characteristics of the Reflection Nebula NGC 2023","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Reflection nebula; Nebula; Emission spectrum; Interstellar medium; Spectral resolution; Infrared; Spectrograph; Spectral line; Reflection (computer programming)","score_opus":0.015081096696503515,"score_gpt":0.27529466791373797,"score_spread":0.26021357121723443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2580872109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99868864,0.00003635109,0.00019427811,0.000011142868,6.1751365e-7,0.0000020486184,0.0001974424,0.000050435392,0.0008191396],"genre_scores_gemma":[0.9992618,0.000013348186,0.0002588486,0.0000071678983,0.0000012001262,0.0000018942462,0.0003465913,0.0000062606987,0.00010277783],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999695,0.0000023040182,0.0000013061039,0.000008585418,0.000009643597,0.000008634437],"domain_scores_gemma":[0.99991524,0.000013466283,0.00002500095,0.00000760959,0.000015001136,0.000023574456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000067082714,0.00018303853,0.00011763034,0.00041526748,0.0002472027,0.0001635428,0.00017761604,0.00017702833,0.00096266455],"category_scores_gemma":[0.000103186416,0.000101795005,0.00019662555,0.00025000362,0.00013815616,0.00008035146,0.00012573601,0.00012879595,0.00021841776],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004325657,0.00008944163,0.4709646,0.00004809761,0.00008199957,0.0009887307,0.00027816684,0.0058759097,0.50727236,0.00037584323,0.00090066955,0.012691568],"study_design_scores_gemma":[0.000011398445,0.000050781142,0.9865866,0.0000030297467,0.000012821007,0.00034933756,0.00007463995,0.005757678,0.006568207,0.000088773515,0.0004891119,0.000007644757],"about_ca_topic_score_codex":0.007139087,"about_ca_topic_score_gemma":0.0075460584,"teacher_disagreement_score":0.007139087,"about_ca_system_score_codex":0.00023724408,"about_ca_system_score_gemma":0.0000816561,"threshold_uncertainty_score":0.014195085},"labels":[],"label_agreement":null},{"id":"W2580880899","doi":"10.3847/1538-4357/836/1/67","title":"Galactic Dark Matter Halos and Globular Cluster Populations. III. Extension to Extreme Environments","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":156,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Globular cluster; Galaxy; Dark matter; Milky Way; Galaxy cluster; Galaxy groups and clusters; Cluster (spacecraft); Dark matter halo; Halo","score_opus":0.01718619030113417,"score_gpt":0.232172181546712,"score_spread":0.21498599124557782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2580880899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99601316,0.0006191765,0.0002906057,0.00023170853,0.0000042953325,0.0000029946298,0.00011773219,0.000010051846,0.0027103361],"genre_scores_gemma":[0.9996327,0.00009173564,0.00004074286,0.000019470253,0.0000058803007,7.1537863e-7,0.0000467953,0.000002484449,0.00015943641],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979,0.00007413075,0.0000071677346,0.000038492875,0.000022340153,0.00006793984],"domain_scores_gemma":[0.99691284,0.0011631149,0.0006695643,0.00030315307,0.00019414604,0.00075715047],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009596523,0.00027014696,0.0003112609,0.0010798969,0.00047140665,0.0009392858,0.00038340272,0.00044721377,0.002586274],"category_scores_gemma":[0.0025946493,0.00017098639,0.0005348119,0.0008390117,0.0010772629,0.00085853203,0.0019374838,0.00078845856,0.00025421576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017192934,0.00002675059,0.98514974,0.000023718974,0.0001740783,0.000304177,0.00023587656,0.0034650078,0.0008407435,0.0031748426,0.00031922042,0.0061139734],"study_design_scores_gemma":[0.000005217274,0.000031364543,0.99484223,0.000015523423,0.000038318052,0.00016903316,0.00034927187,0.001824687,0.00015642423,0.0021462578,0.00041331985,0.000008371496],"about_ca_topic_score_codex":0.0047036936,"about_ca_topic_score_gemma":0.0038373875,"teacher_disagreement_score":0.0047036936,"about_ca_system_score_codex":0.00028382897,"about_ca_system_score_gemma":0.00014540917,"threshold_uncertainty_score":0.009352624},"labels":[],"label_agreement":null},{"id":"W2581675082","doi":"10.3847/1538-4357/aa5b84","title":"A Principal Component Analysis of the Diffuse Interstellar Bands","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Principal component analysis; Component (thermodynamics); Interstellar medium; Physics; Astrobiology; Astronomy; Astrophysics; Computer science; Artificial intelligence; Galaxy","score_opus":0.014972168426545016,"score_gpt":0.25602988396112575,"score_spread":0.24105771553458072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2581675082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.909526,0.0003710428,0.07885397,0.00020483836,0.000122107,0.00029192137,0.0052044066,0.0010587347,0.0043669585],"genre_scores_gemma":[0.95282376,0.00028094306,0.03895293,0.000018333929,0.00005541406,0.00015516259,0.005210689,0.00011211705,0.0023906138],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99949265,0.00008530998,0.000026026688,0.00013817786,0.00018586594,0.00007204768],"domain_scores_gemma":[0.99923754,0.00018093694,0.00007270819,0.00008038759,0.00036920622,0.000059297785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006171827,0.000934191,0.0004275646,0.0020765776,0.00047823729,0.00112402,0.00024610586,0.0001765516,0.0030989677],"category_scores_gemma":[0.0017390721,0.00012678852,0.00078664284,0.0025284307,0.00028150002,0.0002712464,0.00043704288,0.00046657512,0.0007551364],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071072363,0.0005969465,0.17453656,0.00026950042,0.00080826966,0.00035489956,0.00077284593,0.023980204,0.062611386,0.0036567303,0.0129480595,0.71875393],"study_design_scores_gemma":[0.000042439176,0.00027142596,0.8650875,0.000047772108,0.0002468358,0.00021881274,0.0006917043,0.11012774,0.009547941,0.0024539214,0.011150938,0.00011300558],"about_ca_topic_score_codex":0.009350982,"about_ca_topic_score_gemma":0.0050670174,"teacher_disagreement_score":0.009350982,"about_ca_system_score_codex":0.00031778982,"about_ca_system_score_gemma":0.00070575794,"threshold_uncertainty_score":0.018593132},"labels":[],"label_agreement":null},{"id":"W2581974067","doi":"10.3847/1538-4357/aa65d0","title":"The SCUBA-2 Cosmology Legacy Survey: Multi-wavelength Properties of ALMA-identified Submillimeter Galaxies in UKIDSS UDS","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":141,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Aspen Center for Physics; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Photometric redshift; Spectral energy distribution; Luminous infrared galaxy; Infrared; Population; Astronomy; Wavelength; Luminosity; Optics","score_opus":0.03068148978838796,"score_gpt":0.2485788884797133,"score_spread":0.21789739869132535,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2581974067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989065,0.000057016303,0.000044062777,0.000007876925,0.0000012991284,0.000003999796,0.0006188905,0.000008301952,0.0003520663],"genre_scores_gemma":[0.99825066,0.000027248492,0.00013085901,0.00001360527,0.0000048581687,0.0000060040684,0.0013712181,0.000003164284,0.00019241267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997693,0.00003354839,0.000022259814,0.00006565399,0.00005168326,0.000057499303],"domain_scores_gemma":[0.9989518,0.000109818255,0.00040220792,0.00015158157,0.00016886827,0.00021567149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002679052,0.00026168785,0.00024385864,0.0024285861,0.00035361102,0.000619296,0.00034155187,0.00018254615,0.0011612927],"category_scores_gemma":[0.00092798425,0.00016334472,0.00021493467,0.001231224,0.0002680764,0.00032533068,0.00090518047,0.00016201955,0.00043933108],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046362427,0.00001505729,0.9952325,0.000007977763,0.00002141473,0.000047282796,0.00016597514,0.00005961729,0.002249429,0.000034009037,0.00024149354,0.0018789234],"study_design_scores_gemma":[0.0000014195748,0.0000064508404,0.9995229,0.000002288504,0.0000029058917,0.000040164938,0.00005684002,0.000097446,0.000115598545,0.000005481157,0.00014737176,0.0000011051875],"about_ca_topic_score_codex":0.017775835,"about_ca_topic_score_gemma":0.029567562,"teacher_disagreement_score":0.017775835,"about_ca_system_score_codex":0.00035812004,"about_ca_system_score_gemma":0.00014263015,"threshold_uncertainty_score":0.03534472},"labels":[],"label_agreement":null},{"id":"W2582193108","doi":"10.3847/1538-4357/aa5b97","title":"On Integral Upper Limits Assuming Power-law Spectra and the Sensitivity in High-energy Astronomy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Limit (mathematics); Sensitivity (control systems); Spectral line; Parameter space; Astroparticle physics; Space (punctuation); Spectrum (functional analysis); Simple (philosophy); Universe","score_opus":0.00599296655500908,"score_gpt":0.23192393502425523,"score_spread":0.22593096846924615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2582193108","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1884747,0.0038913004,0.7323755,0.003450047,0.00033803063,0.00006108654,0.00017814322,0.00083136704,0.07039982],"genre_scores_gemma":[0.95591736,0.0013148232,0.03969203,0.0005019828,0.0006495964,0.00006639441,0.00009805479,0.00020906566,0.0015506016],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99435896,0.0025981239,0.00022953971,0.001116389,0.0013412852,0.00035580687],"domain_scores_gemma":[0.9016062,0.08175785,0.005367761,0.0078631155,0.0020215693,0.0013834912],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010257259,0.0012388671,0.0014633887,0.0037136127,0.0010840549,0.003596491,0.003080444,0.0018212654,0.0050455937],"category_scores_gemma":[0.08067798,0.0006371563,0.001405215,0.0016799681,0.010957831,0.0121992,0.005998928,0.0049982085,0.000644075],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039407034,0.000052244035,0.0035392807,0.00013654774,0.000036150337,0.00038377073,0.000323164,0.011255333,0.0016567429,0.97086424,0.0007691723,0.010944059],"study_design_scores_gemma":[0.000005679159,0.000025178451,0.0017280653,0.000065790904,0.00001364372,0.00036072623,0.00004435591,0.05136544,0.00094146346,0.94454384,0.00087529584,0.000030457008],"about_ca_topic_score_codex":0.0005882899,"about_ca_topic_score_gemma":0.00024292692,"teacher_disagreement_score":0.010257259,"about_ca_system_score_codex":0.001340337,"about_ca_system_score_gemma":0.00046449367,"threshold_uncertainty_score":0.054246247},"labels":[],"label_agreement":null},{"id":"W2582235831","doi":"10.3847/1538-4357/835/2/265","title":"Dense Molecular Gas Tracers in the Outflow of the Starburst Galaxy NGC 253","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Outflow; Galaxy; Line (geometry); Velocity dispersion; Luminosity; Hubble sequence; Ionization; Active galactic nucleus; Star formation","score_opus":0.010820991471213777,"score_gpt":0.24661539321479642,"score_spread":0.23579440174358265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2582235831","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991073,0.000101745434,0.0003848341,0.0000050614585,9.963733e-7,0.000002159016,0.000058517486,0.000028039833,0.0003114411],"genre_scores_gemma":[0.9993525,0.000025897492,0.00048112954,0.0000040711307,0.0000012006291,0.0000016969685,0.0000555317,0.0000034007912,0.00007460373],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996233,0.00000539551,0.0000025015236,0.000011811949,0.000008866573,0.000009098418],"domain_scores_gemma":[0.9998841,0.000026984884,0.00003807297,0.000013281266,0.000010792589,0.000026716425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014430554,0.00016726696,0.00022084353,0.00037994864,0.00021084766,0.00033784716,0.00024963252,0.00019000961,0.0006583234],"category_scores_gemma":[0.00017375924,0.000094178125,0.00017939895,0.00018881814,0.00013099582,0.00016368415,0.00018020284,0.0001008724,0.000116121366],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033191414,0.00012175253,0.42942598,0.00007385185,0.00012444098,0.0009534241,0.00028983562,0.010507713,0.5497697,0.000572755,0.000118694974,0.0077098645],"study_design_scores_gemma":[0.000025124255,0.00031567574,0.91845703,0.000016335214,0.00008463641,0.00040871938,0.00020258562,0.0371601,0.041405845,0.00034708375,0.0015544242,0.000022491746],"about_ca_topic_score_codex":0.002864292,"about_ca_topic_score_gemma":0.003314024,"teacher_disagreement_score":0.002864292,"about_ca_system_score_codex":0.00037754286,"about_ca_system_score_gemma":0.00007157801,"threshold_uncertainty_score":0.0056952834},"labels":[],"label_agreement":null},{"id":"W2582609153","doi":"10.3847/1538-4357/aa7d57","title":"A Search for Fast Radio Bursts with the GBNCC Pulsar Survey","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Precursory Research for Embryonic Science and Technology; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; European Commission; National Science Foundation","keywords":"Pulsar; Spectral index; Physics; Astrophysics; Flux (metallurgy); Sky; Pulse (music); Scattering; Fast radio burst; Spectral line; Astronomy; Detector; Optics; Galaxy","score_opus":0.02832442896779186,"score_gpt":0.3467254646617934,"score_spread":0.3184010356940015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2582609153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99784446,0.00007955507,0.00078839343,0.000074350486,0.000003510928,0.000010491395,0.00042563706,0.000040629115,0.000732916],"genre_scores_gemma":[0.9977042,0.000040518706,0.00143406,0.00002423496,0.000005067575,0.0000057325537,0.0006478562,0.000008956688,0.00012930509],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971,0.00009556325,0.000007637994,0.000061635816,0.00007303473,0.00005203315],"domain_scores_gemma":[0.9990747,0.0003679042,0.00017392657,0.000090729285,0.00009910973,0.00019369983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077357364,0.00025691334,0.00024636107,0.0005992402,0.00041999028,0.0006399921,0.0003723648,0.00028132883,0.0009485237],"category_scores_gemma":[0.0016239401,0.00018847783,0.00026770402,0.0007247356,0.00024068738,0.00021615997,0.00032811033,0.00026803347,0.0001538215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018214507,0.00006544622,0.96209455,0.00002664139,0.0001367987,0.00025310804,0.00011090029,0.02374146,0.003611539,0.00089890044,0.0011695029,0.0077090412],"study_design_scores_gemma":[0.00008037034,0.00018143872,0.85699064,0.000021727996,0.00009082588,0.00024304549,0.000151159,0.13682716,0.0018873992,0.0007036428,0.002794721,0.000027924296],"about_ca_topic_score_codex":0.030262085,"about_ca_topic_score_gemma":0.03452541,"teacher_disagreement_score":0.030262085,"about_ca_system_score_codex":0.000780031,"about_ca_system_score_gemma":0.0004808662,"threshold_uncertainty_score":0.060171902},"labels":[],"label_agreement":null},{"id":"W2582693918","doi":"10.3847/1538-4357/aa5b95","title":"The JCMT Gould Belt Survey: A First Look at IC 5146","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Manitoba; University of Alberta; Université Laval; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; University of Waterloo; McMaster University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Compute Canada; Canarie; Canadian Foundation for AIDS Research; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Protostar; Astrophysics; Physics; Orion Nebula; Nebula; Extinction (optical mineralogy); Star formation; Molecular cloud; Astronomy; Stars; Optics","score_opus":0.01993324103001388,"score_gpt":0.26193852654921124,"score_spread":0.24200528551919737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2582693918","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950635,0.00034721039,0.000050598897,0.0001317733,0.0000036646481,0.000015117706,0.0025031916,0.00002105885,0.001863873],"genre_scores_gemma":[0.9960743,0.00030697926,0.000195342,0.00009658968,0.000013991685,0.000008439712,0.002306474,0.00000817778,0.0009896922],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998084,0.000011947864,0.000011000423,0.000047793044,0.00005424325,0.00006670354],"domain_scores_gemma":[0.9996278,0.000015104013,0.00014181081,0.00003283777,0.00004776018,0.00013464011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000113621696,0.00015979137,0.00020401903,0.0026703533,0.00067535066,0.0005446868,0.00022584466,0.00028010868,0.0032432834],"category_scores_gemma":[0.0004167898,0.00011849293,0.00015262667,0.0018829897,0.00019875684,0.0003375045,0.0006555198,0.0001557526,0.00051225274],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031409432,0.000014311701,0.9877487,0.000029674733,0.000016343976,0.00029128385,0.0005301454,0.000042993714,0.0045315675,0.00006125605,0.00090116984,0.0058011306],"study_design_scores_gemma":[6.4133104e-7,0.0000045890138,0.99895906,0.000003316495,0.000001913529,0.00009146911,0.00008027901,0.000016467602,0.00005849653,0.0000035884866,0.0007792363,9.026484e-7],"about_ca_topic_score_codex":0.08001678,"about_ca_topic_score_gemma":0.16531712,"teacher_disagreement_score":0.08001678,"about_ca_system_score_codex":0.00060452614,"about_ca_system_score_gemma":0.00032103993,"threshold_uncertainty_score":0.15910208},"labels":[],"label_agreement":null},{"id":"W2583081203","doi":"10.3847/1538-4357/835/2/166","title":"A Type II Supernova Hubble Diagram from the CSP-I, SDSS-II, and SNLS Surveys*","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"Science and Technology Facilities Council; Jet Propulsion Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Centre National de la Recherche Scientifique; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Consejo Nacional de Investigaciones Científicas y Técnicas; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Dark energy; Supernova; Redshift; Cosmic distance ladder; Hubble's law; Diagram; Sky; Cosmology","score_opus":0.019729130158325586,"score_gpt":0.253161284004974,"score_spread":0.23343215384664842,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2583081203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9775054,0.00032090402,0.011245674,0.000036294194,0.000013469318,0.000029023724,0.00482095,0.00024075595,0.0057874685],"genre_scores_gemma":[0.9907107,0.00006283925,0.0047587105,0.000006192436,0.00000644081,0.00000996494,0.004147723,0.000017763985,0.0002797132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997496,0.000074407384,0.000020957585,0.00005935522,0.00006706932,0.000028517103],"domain_scores_gemma":[0.9990101,0.00024261234,0.00020088963,0.00014649889,0.00025248728,0.00014741307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007177472,0.00023294099,0.00019277153,0.0036082629,0.00019741002,0.00058384775,0.0001817008,0.00015571962,0.00228371],"category_scores_gemma":[0.0014554954,0.00007875658,0.0002564684,0.0012889206,0.00015355361,0.00034829965,0.00051059097,0.00017293924,0.00038854085],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020240685,0.00003812132,0.95020044,0.00006429744,0.00012609904,0.000081727296,0.000109929955,0.0056593167,0.0046583824,0.004397704,0.001541459,0.03292018],"study_design_scores_gemma":[0.000012107967,0.00007456298,0.9723318,0.000023633607,0.00004241079,0.00018577364,0.00011394463,0.017338753,0.002021886,0.0026269148,0.005216313,0.000011830058],"about_ca_topic_score_codex":0.004335069,"about_ca_topic_score_gemma":0.0048875134,"teacher_disagreement_score":0.004335069,"about_ca_system_score_codex":0.00030142567,"about_ca_system_score_gemma":0.00028149868,"threshold_uncertainty_score":0.008619666},"labels":[],"label_agreement":null},{"id":"W2583301693","doi":"10.3847/1538-4357/836/1/137","title":"Structural and Photometric Properties of the Andromeda Satellite Dwarf Galaxy Lacerta I from Deep Imaging with WIYN pODI","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Photometry (optics); Andromeda Galaxy; Surface brightness; Andromeda; Galaxy; Dwarf galaxy; Red-giant branch; Population","score_opus":0.009228349603181146,"score_gpt":0.20142615105000441,"score_spread":0.19219780144682327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2583301693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99589914,0.000098973134,0.0008558977,0.000019491625,0.0000013522025,0.0000069767084,0.0008770324,0.00008440324,0.002156722],"genre_scores_gemma":[0.99649507,0.000067193,0.0011989644,0.00001258671,0.0000038899025,0.000004566271,0.0017123069,0.000019601088,0.00048581054],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998909,0.0000058148353,0.000004244264,0.000035402325,0.0000333891,0.000030126275],"domain_scores_gemma":[0.99972945,0.00002197094,0.00008504099,0.00004148268,0.000048843827,0.000073170566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019326899,0.00022786226,0.0001586766,0.0010319842,0.00020983946,0.0005836886,0.00021479884,0.00010409743,0.0006488953],"category_scores_gemma":[0.00029132422,0.00013329221,0.00017885069,0.0004985815,0.00019591571,0.00021207251,0.0004948702,0.00015994441,0.00024018969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019090953,0.000063027794,0.83066446,0.000044769884,0.0000970756,0.00031232502,0.0004536199,0.0018509576,0.13108914,0.00045636916,0.0009060984,0.033871233],"study_design_scores_gemma":[0.0000044958456,0.000024196215,0.9900913,0.0000065159506,0.000025776888,0.00014554326,0.00013926443,0.0022012603,0.0059183235,0.00007110199,0.0013624846,0.00000972719],"about_ca_topic_score_codex":0.011626713,"about_ca_topic_score_gemma":0.02715971,"teacher_disagreement_score":0.011626713,"about_ca_system_score_codex":0.0004152004,"about_ca_system_score_gemma":0.00011459259,"threshold_uncertainty_score":0.023118079},"labels":[],"label_agreement":null},{"id":"W2584386789","doi":"10.3847/1538-4357/aa5ebc","title":"The MASSIVE Survey. VI. The Spatial Distribution and Kinematics of Warm Ionized Gas in the Most Massive Local Early-type Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Kinematics; Stars; Ionization; Equivalent width; Line (geometry); Emission spectrum; Stellar kinematics; Stellar mass","score_opus":0.009829311390956202,"score_gpt":0.22971464112069923,"score_spread":0.21988532972974303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2584386789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99838984,0.0001413293,0.000125049,0.000015501742,0.0000012569765,0.0000049948576,0.0006039883,0.000026860122,0.0006912425],"genre_scores_gemma":[0.99816364,0.000084842875,0.0003319434,0.000013554032,0.000008558707,0.0000048061856,0.00090708036,0.0000060966972,0.0004794201],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998067,0.000029811026,0.000012528518,0.000053275893,0.000040585353,0.00005708173],"domain_scores_gemma":[0.99906534,0.000053961452,0.00040596531,0.000097487435,0.00006453575,0.00031262095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039932042,0.00033201659,0.00022725518,0.0018322713,0.00039493968,0.00049031,0.00032694376,0.00016370101,0.0018111452],"category_scores_gemma":[0.00057984155,0.00017257058,0.00021801621,0.0009047601,0.00029863758,0.00028948442,0.00083518773,0.00015027093,0.0005781402],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007840672,0.000016399463,0.98265517,0.00002267358,0.00003756969,0.00007890946,0.00032201767,0.00008557662,0.008485889,0.00010478399,0.00035796946,0.00775466],"study_design_scores_gemma":[0.0000034757304,0.000029791614,0.9989365,0.0000028268594,0.000011473319,0.000074426665,0.00006156117,0.000052865882,0.00030011288,0.000018368983,0.0005069842,0.0000016730836],"about_ca_topic_score_codex":0.004425997,"about_ca_topic_score_gemma":0.010908771,"teacher_disagreement_score":0.004425997,"about_ca_system_score_codex":0.00029406423,"about_ca_system_score_gemma":0.00013808004,"threshold_uncertainty_score":0.008800507},"labels":[],"label_agreement":null},{"id":"W2584499523","doi":"10.3847/1538-4357/aa67a0","title":"SN 1986J VLBI. III. The Central Component Becomes Dominant","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Very-long-baseline interferometry; RADIUS; Supernova; Quasar; Interferometry; Shell (structure); Flux (metallurgy); Range (aeronautics); Full width at half maximum","score_opus":0.01348252974965765,"score_gpt":0.24394733269477967,"score_spread":0.230464802945122,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2584499523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9722415,0.0005034865,0.0046031587,0.00013481536,0.00004835155,0.00004695555,0.006619793,0.0006243026,0.015177631],"genre_scores_gemma":[0.9687348,0.00015151585,0.00578033,0.000089915746,0.000028722441,0.000014150718,0.016382944,0.000105182226,0.0087124035],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999089,0.0000037423324,0.0000027407518,0.000026387925,0.000026446272,0.00003173937],"domain_scores_gemma":[0.9999076,0.0000027381643,0.00002848725,0.000009551557,0.000020425603,0.0000312706],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015469168,0.00029404627,0.00024539194,0.00076388754,0.00025622742,0.0005649315,0.00015804498,0.00018904387,0.002335386],"category_scores_gemma":[0.0001323334,0.00023120051,0.0002515928,0.00041005993,0.00008877259,0.00014077433,0.00030077546,0.0002450985,0.0011705518],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010265941,0.00019088473,0.61378986,0.00016877489,0.0002617277,0.0009161183,0.00023226828,0.0025133875,0.28188154,0.0013826062,0.011159372,0.08647682],"study_design_scores_gemma":[0.0000090350195,0.000024141824,0.9852933,0.0000082347515,0.000023927854,0.00042751883,0.000033702167,0.0020850124,0.006398012,0.00007472639,0.0056161922,0.000006220685],"about_ca_topic_score_codex":0.017442264,"about_ca_topic_score_gemma":0.037432294,"teacher_disagreement_score":0.017442264,"about_ca_system_score_codex":0.0004973419,"about_ca_system_score_gemma":0.00024299618,"threshold_uncertainty_score":0.03468144},"labels":[],"label_agreement":null},{"id":"W2585286720","doi":"10.3847/1538-4357/835/2/203","title":"A GALACTIC MOLECULAR CLOUD CLUMP CATALOG FROM HI-GAL DATA: METHOD AND INITIAL RESULTS COMPARISON WITH BGPS","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galactic plane; Molecular cloud; Confusion; Galaxy; Disc; Galactic Center; Active galactic nucleus; Range (aeronautics)","score_opus":0.03524592989630737,"score_gpt":0.33176796707110084,"score_spread":0.2965220371747935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2585286720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9539066,0.00044862734,0.019974077,0.0000911885,0.000041488176,0.00082616374,0.017618071,0.002754947,0.0043388274],"genre_scores_gemma":[0.87168914,0.0002692997,0.0669795,0.00007314983,0.00006058894,0.0004707235,0.05810013,0.00048508449,0.0018723222],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99875236,0.00032501126,0.000114750845,0.00029446927,0.00038486108,0.00012856792],"domain_scores_gemma":[0.9965127,0.0006052183,0.00022742324,0.0010241296,0.0013412054,0.00028942546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022705498,0.0004330513,0.0003712649,0.005551054,0.00041153686,0.0014646909,0.001008849,0.0004159188,0.0023682073],"category_scores_gemma":[0.0054460326,0.00021830075,0.00039010632,0.0030262894,0.00021343122,0.00093675393,0.0014892451,0.00028547767,0.0018573914],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009848803,0.00035380435,0.8154686,0.00019508658,0.00018739013,0.0002996228,0.00042317348,0.0048825005,0.010740589,0.00047092958,0.0049243364,0.1610691],"study_design_scores_gemma":[0.0002165415,0.000430132,0.92820364,0.00005891895,0.00015822133,0.00034026988,0.0010107699,0.04425841,0.012547243,0.00032098603,0.012390673,0.000064226995],"about_ca_topic_score_codex":0.012723972,"about_ca_topic_score_gemma":0.009638635,"teacher_disagreement_score":0.012723972,"about_ca_system_score_codex":0.0005101142,"about_ca_system_score_gemma":0.00048010657,"threshold_uncertainty_score":0.025299847},"labels":[],"label_agreement":null},{"id":"W2585531409","doi":"10.3847/1538-4357/aa9576","title":"How to Reconcile the Observed Velocity Function of Galaxies with Theory","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Dark matter; Dwarf galaxy problem; Dwarf galaxy; Halo; Dwarf spheroidal galaxy; Cold dark matter; Astronomy; Galaxy group; Dark matter halo; Galaxy formation and evolution","score_opus":0.01778641735870146,"score_gpt":0.20761043423070846,"score_spread":0.189824016872007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2585531409","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78943455,0.0002894401,0.2002614,0.004077947,0.00014717327,0.000020236452,0.00032251386,0.0008611095,0.004585606],"genre_scores_gemma":[0.9844946,0.00004554716,0.014886143,0.0002203043,0.000026528813,0.000010401482,0.00010797408,0.00007493261,0.00013353227],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9987902,0.000569635,0.00004867268,0.0002919239,0.00022348431,0.00007605557],"domain_scores_gemma":[0.99269754,0.0032701737,0.0009190476,0.0022532619,0.00063708675,0.00022284116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0040382673,0.0004928192,0.0005004926,0.0009534273,0.0004876958,0.0018521943,0.0014016137,0.00066092535,0.00070268725],"category_scores_gemma":[0.022677377,0.0003705114,0.00041571225,0.00058051816,0.0013395183,0.002648331,0.0008861535,0.0010072816,0.00022073828],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017838871,0.00016486383,0.25281462,0.00016677426,0.00041273248,0.00031345655,0.00074590085,0.5099866,0.011374219,0.17526957,0.003046532,0.045526378],"study_design_scores_gemma":[0.00004167041,0.000089811554,0.030058544,0.00005102596,0.0000397289,0.00015389032,0.0002739376,0.7849995,0.007359734,0.17415474,0.002723137,0.000054293232],"about_ca_topic_score_codex":0.004375331,"about_ca_topic_score_gemma":0.002479059,"teacher_disagreement_score":0.004375331,"about_ca_system_score_codex":0.001430045,"about_ca_system_score_gemma":0.0007124633,"threshold_uncertainty_score":0.021356702},"labels":[],"label_agreement":null},{"id":"W2586752546","doi":"10.3847/1538-4357/aa5f5d","title":"Spectral Energy Distribution and Radio Halo of NGC 253 at Low Radio Frequencies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Jet Propulsion Laboratory; ARC Centre of Excellence for All-Sky Astrophysics; Commonwealth Scientific and Industrial Research Organisation; Australian Government; California Institute of Technology; National Aeronautics and Space Administration; Curtin University of Technology; Astronomy Australia Limited; National Science Foundation","keywords":"Physics; Astrophysics; Synchrotron; Flattening; Radio spectrum; Halo; Spectral energy distribution; Radio galaxy; Synchrotron radiation; Galaxy; Astronomy; Optics","score_opus":0.008419897065767679,"score_gpt":0.21063841412330797,"score_spread":0.2022185170575403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2586752546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99757344,0.00007520784,0.0008989014,0.000021124759,0.0000015950678,0.0000022150393,0.00015554918,0.00005850376,0.0012134914],"genre_scores_gemma":[0.9995932,0.000019559893,0.00012190416,0.0000044974154,0.0000019707222,0.0000011633639,0.00013711974,0.0000062234317,0.00011427528],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999428,0.000007696998,0.000002858324,0.000019021134,0.000013441903,0.000014190265],"domain_scores_gemma":[0.9997731,0.000034405006,0.00006913511,0.000025260022,0.000030989897,0.00006720421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014925291,0.00022859669,0.00020630106,0.00038211065,0.00017015723,0.00039711312,0.00023929572,0.00015277664,0.0012378885],"category_scores_gemma":[0.0003321296,0.00011484879,0.00024852302,0.00022917893,0.0002295124,0.0001466104,0.0001947279,0.00016004937,0.0003572108],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015051632,0.000057927537,0.90765494,0.000022924563,0.00007431173,0.00051039254,0.00012798532,0.025354642,0.05932658,0.000829121,0.00040416763,0.005486546],"study_design_scores_gemma":[0.000011359193,0.00006503876,0.97654414,0.0000091976035,0.000031449457,0.0001960118,0.00010211173,0.019066956,0.002941676,0.00037492707,0.0006407664,0.000016442931],"about_ca_topic_score_codex":0.0076073054,"about_ca_topic_score_gemma":0.005042344,"teacher_disagreement_score":0.0076073054,"about_ca_system_score_codex":0.0005482848,"about_ca_system_score_gemma":0.00009124159,"threshold_uncertainty_score":0.0151260495},"labels":[],"label_agreement":null},{"id":"W2587124709","doi":"10.3847/1538-4357/836/1/23","title":"Gamma-ray Observations of Tycho’s Supernova Remnant with VERITAS and Fermi","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Spectral index; Astrophysics; Fermi Gamma-ray Space Telescope; Supernova remnant; Cosmic ray; Gamma ray; Supernova; Range (aeronautics); Astronomy; Spectral line","score_opus":0.020360798058610904,"score_gpt":0.23577392549741172,"score_spread":0.2154131274388008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2587124709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99561596,0.00017427735,0.00038795228,0.000031099407,0.000008352406,0.000010418666,0.0008633705,0.000102168044,0.0028064935],"genre_scores_gemma":[0.99569124,0.00007025171,0.0012118351,0.000034557954,0.000015924008,0.00000929642,0.002262304,0.00003607089,0.0006686548],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997534,0.0000184476,0.000017041644,0.00005549287,0.00009537474,0.00006019795],"domain_scores_gemma":[0.9990287,0.00007051414,0.0002980214,0.00022401976,0.00020349183,0.00017523064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006410024,0.00029418874,0.0002876894,0.0018999379,0.0005338969,0.0006186957,0.00046042394,0.00030323924,0.0013293815],"category_scores_gemma":[0.000702134,0.00026207787,0.00045468094,0.0010748114,0.00037616567,0.00034589085,0.0012026391,0.00042838053,0.00034195962],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009105943,0.00010187805,0.90996206,0.000057229834,0.00023794197,0.0016301342,0.0009244309,0.00072015706,0.06477706,0.00042665855,0.0013842992,0.018867558],"study_design_scores_gemma":[0.000013607438,0.000069183596,0.99302363,0.000011747517,0.00003486372,0.0003993154,0.00011139826,0.00059012463,0.0038734754,0.00003964776,0.0018237779,0.000009190469],"about_ca_topic_score_codex":0.029640507,"about_ca_topic_score_gemma":0.05622411,"teacher_disagreement_score":0.029640507,"about_ca_system_score_codex":0.0009801548,"about_ca_system_score_gemma":0.00031389072,"threshold_uncertainty_score":0.05893594},"labels":[],"label_agreement":null},{"id":"W2587700805","doi":"10.3847/0004-637x/817/1/74","title":"DISTANCE AND EVOLUTIONARY STATE OF THE SUPERNOVA REMNANT 3C 397 (G41.1-0.3)","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Astrophysics; Supernova remnant; Ejecta; Supernova; Spectral line; Absorption (acoustics); Shock (circulatory); Point source; Astronomy; Optics","score_opus":0.005707716228726114,"score_gpt":0.1975300777822108,"score_spread":0.19182236155348467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2587700805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99966276,0.0000112861835,0.000016064401,0.0000023841806,3.128665e-7,5.868049e-7,0.00007710412,0.0000020656023,0.00022738623],"genre_scores_gemma":[0.9993389,0.000010723491,0.000051932697,0.0000030942529,7.283209e-7,9.766444e-7,0.00045406123,0.0000032912994,0.00013622784],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999467,0.0000038617623,0.0000030572808,0.000017786415,0.000014412686,0.000014113581],"domain_scores_gemma":[0.99976116,0.000034948487,0.00007909092,0.000027724418,0.000042048636,0.000054927183],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012938323,0.00020860664,0.00017685808,0.00053768826,0.00038546673,0.0003660975,0.00022678115,0.00026546256,0.0010973284],"category_scores_gemma":[0.00031237656,0.00008363422,0.00019519262,0.00041756846,0.0002442002,0.00012923132,0.0002713879,0.00015968064,0.0004167288],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063628843,0.00008724158,0.91871285,0.00002176514,0.00008332728,0.001995648,0.00033793505,0.0029781482,0.068584725,0.00045116807,0.00028822484,0.0058225906],"study_design_scores_gemma":[0.000008915558,0.000079468504,0.9923463,0.000003537015,0.000019956091,0.00090876705,0.00020157167,0.0020226075,0.0033787761,0.00013391953,0.00088319735,0.000012961425],"about_ca_topic_score_codex":0.009572749,"about_ca_topic_score_gemma":0.0094636865,"teacher_disagreement_score":0.009572749,"about_ca_system_score_codex":0.00042732296,"about_ca_system_score_gemma":0.00011198161,"threshold_uncertainty_score":0.019034028},"labels":[],"label_agreement":null},{"id":"W2587847012","doi":"10.3847/1538-4357/836/2/155","title":"The Relativistic Jet-accretion Flow–wind Connection in Mrk 231","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Quasar; Flare; Very Long Baseline Array; Astronomy; Brightness; Radio telescope; Blazar; Active galactic nucleus; Galaxy; Gamma ray","score_opus":0.01696177912568035,"score_gpt":0.2525554449391344,"score_spread":0.23559366581345403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2587847012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996301,0.0001006004,0.000037061407,0.000023572991,0.0000028851332,0.0000019771294,0.00003007456,0.0000032626065,0.00017051517],"genre_scores_gemma":[0.99978644,0.000028060149,0.000029407316,0.0000062649415,0.000009817767,0.0000012431378,0.0000427838,8.901327e-7,0.00009507321],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999311,0.0000067693654,0.0000065679305,0.00001757904,0.000013625223,0.000024396166],"domain_scores_gemma":[0.9997205,0.000028715847,0.00014672377,0.000014258116,0.00002181004,0.0000679694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012373946,0.0001461073,0.00017198315,0.00046211106,0.00027723343,0.0004217968,0.0001924195,0.00022519635,0.0012758535],"category_scores_gemma":[0.00046930165,0.00010134368,0.0001284893,0.00023676139,0.00030497767,0.00014148554,0.00031418476,0.00026572286,0.00023778804],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003240874,0.00013698549,0.9456044,0.00002954737,0.000048436035,0.0057517462,0.00034892643,0.00023159076,0.038864847,0.00019501972,0.00020446819,0.008259928],"study_design_scores_gemma":[0.0000058733467,0.00009281063,0.99657935,0.0000021931924,0.00001070242,0.0023185716,0.000104089384,0.00016600158,0.00044922513,0.000064255684,0.0002024155,0.0000044794238],"about_ca_topic_score_codex":0.00225648,"about_ca_topic_score_gemma":0.001788341,"teacher_disagreement_score":0.00225648,"about_ca_system_score_codex":0.00026738108,"about_ca_system_score_gemma":0.00012889571,"threshold_uncertainty_score":0.0044866204},"labels":[],"label_agreement":null},{"id":"W2588052779","doi":"10.3847/1538-4357/836/1/147","title":"Erratum: “The Next Generation Virgo Cluster Survey. X. Properties of Ultra-compact Dwarfs in the M87, M49, and M60 Regions” (2015, APJ, 812, 34)","year":2017,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Virgo Cluster; Astrophysics; Cluster (spacecraft); Galaxy; Astronomy; Galaxy cluster; Operating system","score_opus":0.05932159618638213,"score_gpt":0.261527308603171,"score_spread":0.2022057124167889,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2588052779","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0010325006,0.0010460127,0.00026747843,0.057047218,0.90288335,0.00005802794,0.01784358,0.00063687516,0.019185005],"genre_scores_gemma":[0.015255222,0.005130832,0.0026964857,0.089206025,0.16713986,0.00024189678,0.051807072,0.0022322629,0.6662903],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9984869,0.00010987041,0.00028261586,0.0001776847,0.0007992862,0.00014372915],"domain_scores_gemma":[0.99158317,0.0011411903,0.00070899713,0.0005558954,0.005409197,0.0006015749],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012996583,0.0015362309,0.0012710262,0.0039344146,0.0031458207,0.002734214,0.0018848877,0.0030549588,0.05539774],"category_scores_gemma":[0.0130103715,0.00073896535,0.0010668875,0.0023842654,0.0010982847,0.0020559407,0.00169935,0.005127203,0.045430392],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000014629616,0.000006852566,0.00014594715,0.000023694723,0.000002541669,0.000054339755,0.000006177696,0.000016957934,0.000023166682,0.00015743206,0.997964,0.0015842587],"study_design_scores_gemma":[0.000038820115,0.000027201406,0.0051887077,0.0002035356,0.000021671553,0.00018885877,0.00012301681,0.00012652356,0.0003576229,0.00074661965,0.99294066,0.00003689374],"about_ca_topic_score_codex":0.043268103,"about_ca_topic_score_gemma":0.05697006,"teacher_disagreement_score":0.05539774,"about_ca_system_score_codex":0.0031636234,"about_ca_system_score_gemma":0.0054132477,"threshold_uncertainty_score":0.18532395},"labels":[],"label_agreement":null},{"id":"W2588975167","doi":"10.3847/1538-4357/aa5f54","title":"Polycyclic Aromatic Hydrocarbon Emission in Spitzer/IRS Maps. II. A Direct Link between Band Profiles and the Radiation Field Strength","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Polycyclic aromatic hydrocarbon; Field (mathematics); Field strength; Astrophysics; Link (geometry); Radiation; Astrobiology; Optics; Magnetic field; Quantum mechanics","score_opus":0.007973488588353476,"score_gpt":0.2408067270892388,"score_spread":0.23283323850088533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2588975167","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984074,0.000065683154,0.00047394837,0.0000097089105,9.553005e-7,0.0000034392608,0.0002438264,0.000029262308,0.00076573505],"genre_scores_gemma":[0.99885845,0.000035256224,0.00033837554,0.000004919249,0.0000033726128,0.00000296132,0.00062578527,0.000012221325,0.00011866985],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998791,0.0000139221875,0.000006910424,0.000030253204,0.00003939817,0.000030298563],"domain_scores_gemma":[0.999382,0.00014062945,0.000219594,0.000074118456,0.00011976261,0.00006391519],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020672461,0.0002695403,0.00014779576,0.001547917,0.00013632227,0.00041155907,0.00021103733,0.00022354785,0.0008753798],"category_scores_gemma":[0.00064713886,0.00017796321,0.00024575298,0.0005916212,0.00026738108,0.00041634977,0.0003792184,0.00017040354,0.0004246224],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030554555,0.000063983316,0.86187625,0.000051646937,0.00013302181,0.00016276861,0.00015271692,0.0027849402,0.1181046,0.00044023345,0.00023494067,0.015689325],"study_design_scores_gemma":[0.0000022464567,0.000017531242,0.99514115,0.0000022245745,0.000015543286,0.00006480794,0.000038855982,0.0017699166,0.002703222,0.00010398419,0.00013697524,0.0000034708264],"about_ca_topic_score_codex":0.0014553103,"about_ca_topic_score_gemma":0.0016362673,"teacher_disagreement_score":0.001547917,"about_ca_system_score_codex":0.0001721904,"about_ca_system_score_gemma":0.000071826966,"threshold_uncertainty_score":0.0029284358},"labels":[],"label_agreement":null},{"id":"W2589023807","doi":"10.3847/1538-4357/aa5b8e","title":"The Dependence of Cluster Galaxy Properties on the Central Entropy of Their Host Cluster","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Johns Hopkins University; New Mexico State University; Yale University; Vanderbilt University; University of Portsmouth; University of Washington; Science and Technology Facilities Council; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; Jet Propulsion Laboratory; Princeton University; Brookhaven National Laboratory; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; Galaxy cluster; Intracluster medium; Brightest cluster galaxy; Velocity dispersion; Cluster (spacecraft); Galaxy; Astronomy","score_opus":0.012512456293388383,"score_gpt":0.21017239035274302,"score_spread":0.19765993405935464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2589023807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99944156,0.000023293676,0.000115336974,0.0000039991987,5.1678586e-7,8.5269994e-7,0.00008380826,0.000006414399,0.00032431784],"genre_scores_gemma":[0.99982786,0.000005316741,0.000027127055,9.827387e-7,0.0000011714043,3.859387e-7,0.00009355563,0.0000027983556,0.00004068465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981016,0.000035475474,0.000011088179,0.000050837407,0.0000461296,0.000046306217],"domain_scores_gemma":[0.9962006,0.0015768225,0.00077922444,0.00043470314,0.000330311,0.00067826826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003278136,0.00012215386,0.00021893295,0.0012274892,0.000258524,0.0006250601,0.00022022765,0.00017121837,0.0016750084],"category_scores_gemma":[0.0032093863,0.000112778886,0.00016034082,0.0005336412,0.00041218096,0.00034086616,0.000575033,0.00019481407,0.0002732539],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000228631,0.000014291591,0.9917551,0.000007383389,0.000061660794,0.0000533208,0.00010257916,0.0009093016,0.004926703,0.0002296594,0.000059028906,0.0016522843],"study_design_scores_gemma":[0.0000015736774,0.000021782822,0.99778855,9.76663e-7,0.000008858917,0.00004559342,0.00003957687,0.0014310082,0.00051839196,0.00009057724,0.00004990738,0.0000031367397],"about_ca_topic_score_codex":0.0021214848,"about_ca_topic_score_gemma":0.0015930845,"teacher_disagreement_score":0.0021214848,"about_ca_system_score_codex":0.00023093152,"about_ca_system_score_gemma":0.000110250934,"threshold_uncertainty_score":0.0056034923},"labels":[],"label_agreement":null},{"id":"W2589340393","doi":"10.3847/1538-4357/aa7740","title":"The Remarkable Similarity of Massive Galaxy Clusters from z ∼ 0 to z ∼ 1.9","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":152,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Argonne National Laboratory; University of Chicago; Smithsonian Astrophysical Observatory; U.S. Department of Energy; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Similarity (geometry); Galaxy; Astrophysics; Physics; Computer science; Artificial intelligence","score_opus":0.009497209790478498,"score_gpt":0.22976827438410236,"score_spread":0.22027106459362386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2589340393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979692,0.000087301625,0.00008344683,0.00004527788,0.0000039081083,0.0000027386614,0.0003073753,0.000018379484,0.001482288],"genre_scores_gemma":[0.9991973,0.00002970856,0.00007559777,0.000017940776,0.0000056265894,0.0000017325652,0.00042612938,0.0000045055617,0.00024152605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983907,0.000008443903,0.0000058022474,0.000058624384,0.00003627941,0.000051726907],"domain_scores_gemma":[0.9993104,0.00006933006,0.00024399713,0.000057225756,0.000086795415,0.00023222208],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017258225,0.00012059626,0.00021898371,0.0013823517,0.00048401303,0.0006479248,0.00029380867,0.00018600891,0.0022734054],"category_scores_gemma":[0.00097056816,0.00013200685,0.00013204174,0.0005518287,0.0003350836,0.0002881855,0.00083607,0.00025093355,0.00042909212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020938223,0.00001903441,0.97312295,0.00001971724,0.00004520791,0.00016756123,0.0007954498,0.0001629862,0.01618638,0.00078921294,0.0008586902,0.007623454],"study_design_scores_gemma":[0.0000011341865,0.0000053898784,0.9994923,0.0000011110303,0.00000209369,0.00004081172,0.000038007707,0.000027350115,0.00009884545,0.000048296522,0.00024339401,0.0000011375316],"about_ca_topic_score_codex":0.0050280415,"about_ca_topic_score_gemma":0.0073117153,"teacher_disagreement_score":0.0050280415,"about_ca_system_score_codex":0.0002781996,"about_ca_system_score_gemma":0.0001471454,"threshold_uncertainty_score":0.009997547},"labels":[],"label_agreement":null},{"id":"W2589449674","doi":"10.3847/1538-4357/aa615b","title":"The Dragonfly Nearby Galaxies Survey. III. The Luminosity Function of the M101 Group","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Luminosity function; Astronomy; Galaxy group; Spiral galaxy; Luminosity; Luminous infrared galaxy","score_opus":0.011111736819830471,"score_gpt":0.2153225443770343,"score_spread":0.20421080755720383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2589449674","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966282,0.000104842504,0.0001147103,0.000051089773,0.0000027686117,0.0000069059524,0.0014599545,0.000016389511,0.0016150357],"genre_scores_gemma":[0.99458164,0.000044818567,0.00027483414,0.000031688727,0.00000621464,0.0000058688615,0.0038674546,0.000004754462,0.0011827443],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998677,0.000015767875,0.0000054979864,0.000043824595,0.00003241411,0.00003479603],"domain_scores_gemma":[0.99952996,0.00004336758,0.00014806025,0.00005161061,0.000050599916,0.00017631185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023270368,0.00021307622,0.00013332246,0.0014929518,0.00032672347,0.0004193904,0.0002569165,0.0002148939,0.0018657235],"category_scores_gemma":[0.00045452343,0.000090544294,0.00012094579,0.0006828396,0.0001863716,0.0002769922,0.00046964243,0.0001540753,0.00068286335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010850321,0.000029814038,0.97971797,0.000016567144,0.000032401,0.00008561368,0.00025388302,0.00012406889,0.0038007642,0.00015767939,0.0017941147,0.013878455],"study_design_scores_gemma":[0.0000028161137,0.000018125938,0.9983588,0.000002776309,0.0000037214095,0.000059380483,0.0000842963,0.0001602405,0.00030599983,0.000014421534,0.0009875512,0.0000019175768],"about_ca_topic_score_codex":0.020106332,"about_ca_topic_score_gemma":0.041792046,"teacher_disagreement_score":0.020106332,"about_ca_system_score_codex":0.0006200251,"about_ca_system_score_gemma":0.00013042758,"threshold_uncertainty_score":0.039978623},"labels":[],"label_agreement":null},{"id":"W2590002488","doi":"10.3847/0004-637x/832/1/37","title":"ALMA OBSERVATIONS OF Lyα BLOB 1: HALO SUBSTRUCTURE ILLUMINATED FROM WITHIN","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Knut och Alice Wallenbergs Stiftelse; National Science Council; Leverhulme Trust; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Vetenskapsrådet; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"Halo; Surface brightness; Substructure; Galaxy; Submillimeter Array; Radiative transfer; Brightness; Population","score_opus":0.014892219261709855,"score_gpt":0.2223204059338811,"score_spread":0.20742818667217125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2590002488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998681,0.00003999875,0.00015761504,0.000010550782,0.0000014675849,0.0000025660586,0.0002782457,0.000045685145,0.0007829348],"genre_scores_gemma":[0.9991979,0.000014520953,0.00022953062,0.000010039779,0.0000032287026,0.00000236835,0.00037055896,0.000004300011,0.00016759077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999707,0.0000026065234,7.745048e-7,0.0000081133085,0.000008723673,0.000009190034],"domain_scores_gemma":[0.9999052,0.0000062926333,0.000023663688,0.000009364352,0.0000122610445,0.000043161966],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006396606,0.00015604007,0.00014766544,0.00032156467,0.0002675124,0.00027455072,0.00018003384,0.00012909817,0.0010148721],"category_scores_gemma":[0.000121579564,0.000103202845,0.00016039005,0.0002532568,0.00009109137,0.00013828427,0.00022947237,0.00018320388,0.00019093238],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053713954,0.00017549997,0.8330158,0.00006295239,0.00024185341,0.0004991496,0.0005853317,0.005800423,0.14131224,0.0006103281,0.0022079106,0.014951466],"study_design_scores_gemma":[0.000018664201,0.00006085522,0.99114674,0.0000045640722,0.000021984964,0.00007143639,0.000068556445,0.0051441053,0.0021700722,0.00007096082,0.0012152863,0.0000066640832],"about_ca_topic_score_codex":0.012097569,"about_ca_topic_score_gemma":0.025735255,"teacher_disagreement_score":0.012097569,"about_ca_system_score_codex":0.0004067435,"about_ca_system_score_gemma":0.0000959753,"threshold_uncertainty_score":0.024054289},"labels":[],"label_agreement":null},{"id":"W2590222241","doi":"10.3847/1538-4357/aa9375","title":"Bow Ties in the Sky. II. Searching for Gamma-Ray Halos in the Fermi Sky Using Anisotropy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Intergalactic travel; Halo; Active galactic nucleus; Reionization; Population; Fermi Gamma-ray Space Telescope; Galactic halo; Spectral density; Anisotropy","score_opus":0.032952110673500304,"score_gpt":0.29802519914249903,"score_spread":0.26507308846899874,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2590222241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9710052,0.00023260078,0.023728376,0.00007084485,0.0000059857575,0.000012957788,0.0002758291,0.00024122135,0.004426953],"genre_scores_gemma":[0.9955585,0.000058679543,0.0039670127,0.000012612569,0.000008437329,0.000003109552,0.0001282343,0.000017181022,0.00024619026],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998461,0.00002655705,0.000007068719,0.000044542136,0.0000364431,0.000039276598],"domain_scores_gemma":[0.999332,0.00015556502,0.00022248668,0.0001244963,0.00006658884,0.00009871967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034715614,0.00025117624,0.00016389844,0.0018974267,0.0003252894,0.0009036478,0.00021543322,0.00018742589,0.0013897709],"category_scores_gemma":[0.0015737128,0.00020874233,0.00026102227,0.0009268245,0.00036481468,0.00059257867,0.0004891463,0.00021981879,0.00023668648],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004486521,0.000045736942,0.75016576,0.000100486985,0.00020730462,0.000528709,0.00054254517,0.012000384,0.11418592,0.013796869,0.0010662968,0.10691123],"study_design_scores_gemma":[0.00001960325,0.00007714749,0.9105694,0.00003067925,0.00009544713,0.00076286995,0.00034535266,0.056672994,0.017793193,0.010953211,0.0026467885,0.000033236272],"about_ca_topic_score_codex":0.002089295,"about_ca_topic_score_gemma":0.003832438,"teacher_disagreement_score":0.002089295,"about_ca_system_score_codex":0.00026561748,"about_ca_system_score_gemma":0.00016366964,"threshold_uncertainty_score":0.004649222},"labels":[],"label_agreement":null},{"id":"W2590716565","doi":"10.3847/1538-4357/aa6037","title":"Near-infrared Spectroscopy of Five Ultra-massive Galaxies at 1.7 &lt; z &lt; 2.7","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência, Tecnologia e Inovação; Alexander von Humboldt-Stiftung; National Aeronautics and Space Administration; Max-Planck-Institut für Astronomie; Ministerio de Ciencia, Tecnología e Innovación Productiva; Space Telescope Science Institute; National Science Foundation","keywords":"Galaxy; Photometry (optics); Redshift; Stellar population; Population; Star formation; Spectroscopy; Galaxy formation and evolution; Spectral line","score_opus":0.0072289601250379075,"score_gpt":0.22650191149709226,"score_spread":0.21927295137205435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2590716565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995072,0.00001625469,0.00014513273,0.000011238867,0.0000014872115,0.00000474941,0.00010299178,0.000016716807,0.00019431388],"genre_scores_gemma":[0.9992655,0.0000074194068,0.0002521331,0.000018616347,0.0000033030756,0.0000030366593,0.00029963767,0.000002840456,0.00014751391],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997404,0.000037397236,0.000013537394,0.000055801964,0.00006503486,0.00008766767],"domain_scores_gemma":[0.99911135,0.00009676442,0.000194878,0.00009329434,0.00012407439,0.00037964646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000681819,0.00025619444,0.00035704265,0.0012218137,0.0006757846,0.0005155516,0.000474943,0.00036762163,0.0006974124],"category_scores_gemma":[0.00048582358,0.00018823377,0.00027422843,0.0005702839,0.00029896662,0.00021007509,0.0006062141,0.00026715887,0.0002713421],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003310364,0.00029646023,0.9610834,0.000014622819,0.000055770997,0.00034081188,0.00083527237,0.00039123034,0.029928125,0.00016835523,0.00027132613,0.006283717],"study_design_scores_gemma":[0.0000056942786,0.000088663975,0.9980081,0.0000015279519,0.000013007052,0.000065432854,0.00011295642,0.00043755,0.0010686475,0.000015115059,0.00018030047,0.0000031625195],"about_ca_topic_score_codex":0.0062893596,"about_ca_topic_score_gemma":0.010247277,"teacher_disagreement_score":0.0062893596,"about_ca_system_score_codex":0.00041308586,"about_ca_system_score_gemma":0.00012851378,"threshold_uncertainty_score":0.012505531},"labels":[],"label_agreement":null},{"id":"W2590756877","doi":"10.3847/1538-4357/aa5c40","title":"On Differential Rotation and Overshooting in Solar-like Stars","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Agence Nationale de la Recherche","keywords":"Differential rotation; Physics; Astrophysics; Equator; Stars; Rossby number; Rotation (mathematics); Radiative transfer; Planet; Convection; Scaling; Omega; Convection zone; Helioseismology; Latitude; Astronomy; Geometry; Mechanics; Turbulence","score_opus":0.012040255722549553,"score_gpt":0.23676314537754806,"score_spread":0.2247228896549985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2590756877","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99840313,0.00002951493,0.0008870648,0.000023228213,0.0000023161572,0.0000030476426,0.00004472234,0.000024524148,0.0005825332],"genre_scores_gemma":[0.9996929,0.000010209875,0.00021136749,0.0000038024564,6.972719e-7,0.0000011288801,0.000028076314,0.0000058193646,0.000046032877],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999416,0.000014603016,0.0000032233374,0.000014282447,0.000011196607,0.000015067687],"domain_scores_gemma":[0.9996395,0.00012874877,0.0000917088,0.000038029113,0.000036674755,0.00006525355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025031966,0.00025482342,0.00033988472,0.00032913542,0.0003123325,0.0004833093,0.0002736922,0.00033566088,0.000850146],"category_scores_gemma":[0.0011714346,0.00011965653,0.0003167623,0.00028213195,0.00047876843,0.00031645622,0.00041868372,0.00025129435,0.00010767383],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035455133,0.00011858905,0.14466271,0.000067300156,0.00008690793,0.00048368776,0.0003449001,0.8072293,0.03650202,0.0032198867,0.00029196934,0.0066382363],"study_design_scores_gemma":[0.000033363187,0.0001188606,0.049803335,0.0000113252145,0.000015034208,0.000079272824,0.00010837862,0.943513,0.0048184497,0.0011536081,0.00032342153,0.000022012196],"about_ca_topic_score_codex":0.0037944359,"about_ca_topic_score_gemma":0.0023300515,"teacher_disagreement_score":0.0037944359,"about_ca_system_score_codex":0.00042088705,"about_ca_system_score_gemma":0.0001838985,"threshold_uncertainty_score":0.0075446963},"labels":[],"label_agreement":null},{"id":"W2591205962","doi":"10.3847/1538-4357/836/2/205","title":"A Luminous and Isolated Gamma-Ray Flare from the Blazar B2 1215+30","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Office of Science; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Centre National de la Recherche Scientifique; National Science Foundation; Agenzia Spaziale Italiana; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; U.S. Department of Energy; Space Telescope Science Institute; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Istituto Nazionale di Astrofisica; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet","keywords":"Physics; Blazar; Astrophysics; Fermi Gamma-ray Space Telescope; Flare; Crab Nebula; Astronomy; Spectral index; Observatory; Luminosity; Cherenkov radiation; BL Lac object; Gamma ray; Flux (metallurgy); Population; Spectral energy distribution; Galaxy; Spectral line; Detector","score_opus":0.008726119231967576,"score_gpt":0.21757603092480565,"score_spread":0.20884991169283806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2591205962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97333074,0.00022998308,0.00087804586,0.0003773233,0.00007154038,0.000049677077,0.0023445156,0.00038620958,0.022331791],"genre_scores_gemma":[0.99361247,0.00004957769,0.00058603706,0.00025964493,0.00004135282,0.00000913687,0.002747396,0.000041684314,0.0026526237],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999027,0.000003960401,0.0000040921627,0.000028015815,0.00003356301,0.000027676273],"domain_scores_gemma":[0.99985814,0.000011073536,0.000034369004,0.000014704719,0.000015857797,0.00006592429],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008316134,0.00029654373,0.00019611866,0.00060214486,0.00060883857,0.0005011086,0.00024791787,0.0006471993,0.0036897664],"category_scores_gemma":[0.00021273494,0.00013165853,0.00020123312,0.0004482878,0.00020442053,0.00015964302,0.00035274331,0.000433697,0.0007207704],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011838949,0.0005482119,0.3240139,0.00038614584,0.00030284404,0.02166737,0.0012382296,0.0015504654,0.5474803,0.0047455123,0.04165785,0.055225298],"study_design_scores_gemma":[0.00008018511,0.0002742897,0.95609564,0.0000289794,0.000042821015,0.004661566,0.00012530106,0.0012068384,0.012774574,0.00040514025,0.024266383,0.000038371076],"about_ca_topic_score_codex":0.009095921,"about_ca_topic_score_gemma":0.015329277,"teacher_disagreement_score":0.009095921,"about_ca_system_score_codex":0.0005181392,"about_ca_system_score_gemma":0.00015305777,"threshold_uncertainty_score":0.018085897},"labels":[],"label_agreement":null},{"id":"W2591557515","doi":"10.3847/1538-4357/aa6d13","title":"SHARP: A Spatially Higher-order, Relativistic Particle-in-cell Code","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dust and Plasma Wave Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Interpolation (computer graphics); Convergence (economics); Stability (learning theory); Momentum (technical analysis); Energy–momentum relation; Smoothness; Instability; Kinetic energy","score_opus":0.019564118550275754,"score_gpt":0.2531114117869644,"score_spread":0.23354729323668863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2591557515","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04728153,0.00026814616,0.9280913,0.00026163846,0.00021942193,0.00018943533,0.00055695744,0.0097292205,0.013402318],"genre_scores_gemma":[0.33854535,0.00018398285,0.6519106,0.00020812727,0.00005854911,0.00038631455,0.00072124583,0.001275524,0.0067102793],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996954,0.00006706952,0.000019760948,0.000032497566,0.00015079566,0.000034546763],"domain_scores_gemma":[0.9990627,0.0003065206,0.00008988223,0.00019934266,0.0002484136,0.0000930609],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007098158,0.00048508763,0.00048254515,0.00039331493,0.0004255427,0.001030974,0.0022574465,0.00088393525,0.003939044],"category_scores_gemma":[0.002652537,0.00030055217,0.00051773887,0.0005175987,0.000701426,0.0007490576,0.0011136115,0.0013830318,0.0012365922],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022392867,0.00013863001,0.002903281,0.00019558507,0.00007084108,0.00024694952,0.00019757828,0.85153747,0.016090872,0.07512276,0.007944251,0.045327835],"study_design_scores_gemma":[0.000034684126,0.000021537815,0.000109811685,0.0000067788674,0.0000053742297,0.000019382933,0.000006087535,0.991876,0.0021478075,0.0023136341,0.0034510903,0.000007716515],"about_ca_topic_score_codex":0.004477638,"about_ca_topic_score_gemma":0.0036282802,"teacher_disagreement_score":0.004477638,"about_ca_system_score_codex":0.0005191111,"about_ca_system_score_gemma":0.0015277927,"threshold_uncertainty_score":0.013177395},"labels":[],"label_agreement":null},{"id":"W2591687163","doi":"10.3847/1538-4357/aa60c0","title":"Near-Infrared Knots and Dense Fe Ejecta in the Cassiopeia A Supernova Remnant","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cassiopeia A; Ejecta; Supernova remnant; Supernova; Line (geometry); Emission spectrum","score_opus":0.014796472785945874,"score_gpt":0.24765463801335894,"score_spread":0.23285816522741307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2591687163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996897,0.000041669206,0.00005870637,0.0000037197735,9.435246e-7,0.0000018756749,0.000041416042,0.0000035056191,0.0001585187],"genre_scores_gemma":[0.9995647,0.000034062385,0.0001369995,0.0000028222405,0.0000030809047,0.0000016681769,0.00018242255,0.0000011733005,0.00007303645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999248,0.0000066098387,0.0000052164255,0.000026426396,0.00001915349,0.000017736276],"domain_scores_gemma":[0.9996166,0.00004903792,0.00012638675,0.000040606363,0.00004271889,0.0001246123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022331883,0.00024075624,0.00017696655,0.0010013436,0.00038158608,0.00032554785,0.00015232411,0.00020897674,0.00064464763],"category_scores_gemma":[0.0003492103,0.0001650733,0.00023511857,0.00028566932,0.00031586873,0.0001508741,0.00049646664,0.00019240133,0.000108228574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041829012,0.00007302617,0.9478695,0.00002172219,0.00009411173,0.0024477446,0.00027974043,0.00034026502,0.04468314,0.000069083035,0.00010578442,0.0035975932],"study_design_scores_gemma":[0.000005149061,0.00004669321,0.99775827,0.0000028432619,0.000013887756,0.0007733421,0.000061353894,0.00021141442,0.0009956313,0.000018366944,0.00011006764,0.0000029033577],"about_ca_topic_score_codex":0.0036933862,"about_ca_topic_score_gemma":0.0033769286,"teacher_disagreement_score":0.0036933862,"about_ca_system_score_codex":0.00015480557,"about_ca_system_score_gemma":0.000077755794,"threshold_uncertainty_score":0.007343769},"labels":[],"label_agreement":null},{"id":"W2592048703","doi":"10.3847/1538-4357/aa5eb1","title":"Space Telescope and Optical Reverberation Mapping Project. V. Optical Spectroscopic Campaign and Emission-line Analysis for NGC 5548","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":130,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Natural Sciences and Engineering Research Council of Canada; Comisión Nacional de Investigación Científica y Tecnológica; University of California, Santa Barbara; Jet Propulsion Laboratory; National Research Foundation of Korea; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Space Telescope Science Institute; American Academy in Rome; Science and Technology Facilities Council; National Research Foundation; Danmarks Frie Forskningsfond; National Science Foundation; University of Washington; Ministry of Science, ICT and Future Planning; Ohio State University; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Georgia State University; U.S. Department of Energy; California Institute of Technology; Danmarks Grundforskningsfond; Howard Hughes Medical Institute; National Aeronautics and Space Administration","keywords":"Light curve; Lag; Ultraviolet; Reverberation mapping; RADIUS; Time lag; Optical telescope; Luminosity","score_opus":0.024132662139781196,"score_gpt":0.28489334971856867,"score_spread":0.26076068757878745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2592048703","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99401,0.000033173128,0.00053295045,0.000028015203,0.0000064924416,0.000048353973,0.0036597564,0.0001282777,0.0015529967],"genre_scores_gemma":[0.9838843,0.000026078938,0.0033364138,0.000048818238,0.000014958859,0.00007450696,0.0107938545,0.00004123732,0.001779828],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975735,0.000027926413,0.000013351507,0.00006840676,0.00005543078,0.000077553545],"domain_scores_gemma":[0.99934465,0.00004060151,0.00016554273,0.00015522675,0.00012721297,0.00016674439],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004125316,0.00037538508,0.00021963693,0.00110021,0.0005167848,0.00033218187,0.00029886173,0.00020638508,0.0014624477],"category_scores_gemma":[0.00042495935,0.00013973411,0.00025143,0.00042167882,0.0001253864,0.00020012735,0.0003647691,0.00020058603,0.00068482535],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009926851,0.0005807981,0.81858903,0.000052370902,0.00013124773,0.00089659484,0.0010089582,0.001741019,0.12051619,0.00020893791,0.004269883,0.051012333],"study_design_scores_gemma":[0.000026327207,0.00019302873,0.99217343,0.0000026835187,0.000024085448,0.00010802856,0.00007525121,0.0005950996,0.0039250623,0.000017987768,0.0028532,0.00000590071],"about_ca_topic_score_codex":0.026731133,"about_ca_topic_score_gemma":0.041445825,"teacher_disagreement_score":0.026731133,"about_ca_system_score_codex":0.00048996985,"about_ca_system_score_gemma":0.00025429504,"threshold_uncertainty_score":0.05315107},"labels":[],"label_agreement":null},{"id":"W2592371545","doi":"10.3847/1538-4357/837/1/12","title":"The Interstellar Medium in High-redshift Submillimeter Galaxies as Probed by Infrared Spectroscopy<sup>∗</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Max-Planck-Institut für Astronomie; Munich Institute for Astro- and Particle Physics; Centre National de la Recherche Scientifique; KU Leuven; Ministerio de Economía y Competitividad; California Institute of Technology; European Commission; Leverhulme Trust; Key Programme; Bundesministerium für Verkehr, Innovation und Technologie; Centre National d’Etudes Spatiales; Aspen Center for Physics; Danmarks Grundforskningsfond; National Science Foundation; Imperial College London; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; UK Space Agency","keywords":"Physics; Astrophysics; Galaxy; Interstellar medium; Redshift; Spectroscopy; Infrared; Star formation; Luminous infrared galaxy; Photometry (optics); Spectral line; Astronomy; Stars","score_opus":0.005919540384274305,"score_gpt":0.21736564938933822,"score_spread":0.21144610900506391,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2592371545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973786,0.000091550864,0.000119472956,0.000038074137,0.000005016738,0.0000017467929,0.00041995922,0.000019727431,0.0019258865],"genre_scores_gemma":[0.99897873,0.00004631561,0.00023308049,0.000029617178,0.000010412126,0.0000026585622,0.00049117545,0.000004285788,0.00020379745],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999274,0.000008066499,0.000004474406,0.000017846492,0.000021765094,0.000020302126],"domain_scores_gemma":[0.9995733,0.00008787666,0.00019086787,0.00003527271,0.000039698814,0.0000729859],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020275908,0.0001379224,0.00010503521,0.00059013814,0.00020681926,0.00050552137,0.00018524818,0.00018826248,0.0018984093],"category_scores_gemma":[0.0003946911,0.00008334148,0.0001104495,0.00049704383,0.00024904936,0.00036687712,0.00034574498,0.00014447104,0.0003403701],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000098943034,0.00001701556,0.9544635,0.00002128051,0.000031134816,0.00013002209,0.00014773404,0.0004014461,0.03770391,0.00039255296,0.00065681967,0.005935685],"study_design_scores_gemma":[0.0000012993567,0.000008648754,0.9980546,0.000001683145,0.0000055416563,0.000049680184,0.000093352755,0.00017252598,0.0011701887,0.00004549433,0.00039542938,0.0000014169623],"about_ca_topic_score_codex":0.0019231791,"about_ca_topic_score_gemma":0.0048764194,"teacher_disagreement_score":0.0019231791,"about_ca_system_score_codex":0.00020379835,"about_ca_system_score_gemma":0.00007887014,"threshold_uncertainty_score":0.0063508153},"labels":[],"label_agreement":null},{"id":"W2592387297","doi":"10.3847/1538-4357/aa7557","title":"Hubble Space Telescope  Imaging of the Ultra-compact High Velocity Cloud AGC 226067: A Stripped Remnant in the Virgo Cluster","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Virgo Cluster; Stellar population; Galaxy; Luminosity; Metallicity; Dwarf galaxy; Advanced Camera for Surveys; Star cluster; Hubble space telescope","score_opus":0.01104751637845272,"score_gpt":0.25081669359865405,"score_spread":0.23976917722020133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2592387297","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984836,0.000042080537,0.00014823994,0.000011785824,0.0000030228398,0.0000035968976,0.0003930746,0.00002136273,0.00089331175],"genre_scores_gemma":[0.9981919,0.000024598687,0.00049980456,0.000010933813,0.0000056654617,0.0000017216474,0.00090444594,0.0000064954033,0.00035436163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998828,0.0000052803816,0.000005297648,0.000025076479,0.000046136167,0.0000354813],"domain_scores_gemma":[0.99971884,0.000013341448,0.00005569252,0.000028391049,0.00003959573,0.00014413944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010343664,0.00018128841,0.0001756186,0.0012094986,0.0003730756,0.00042967557,0.000353137,0.00024894564,0.0010012415],"category_scores_gemma":[0.0002083361,0.00012004166,0.00023096387,0.000595274,0.00018003744,0.0001408863,0.0003956793,0.00017285053,0.0004378185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063885655,0.0002550295,0.76000327,0.000060929982,0.00014786815,0.0030697815,0.00040581927,0.0021382174,0.2122313,0.00055422937,0.0020841232,0.01841061],"study_design_scores_gemma":[0.0000067425626,0.00003280065,0.99230474,0.000004971042,0.00001578654,0.0005789706,0.00012772964,0.002261904,0.0037194784,0.0000463905,0.0008946153,0.0000057108355],"about_ca_topic_score_codex":0.010811466,"about_ca_topic_score_gemma":0.018597674,"teacher_disagreement_score":0.010811466,"about_ca_system_score_codex":0.000289288,"about_ca_system_score_gemma":0.00018058743,"threshold_uncertainty_score":0.02149707},"labels":[],"label_agreement":null},{"id":"W2592501867","doi":"10.3847/1538-4357/aa7845","title":"Tiny Electromagnetic Explosions","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Magnetic field; Superluminal motion; Lorentz factor; Scattering; Atomic physics; Electron; Thomson scattering; Optics; Nuclear physics; Lorentz transformation","score_opus":0.011648150444921736,"score_gpt":0.23715053189045993,"score_spread":0.2255023814455382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2592501867","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5046691,0.01262084,0.11782209,0.0021424633,0.0022379477,0.00016560545,0.0013997357,0.0014460994,0.3574962],"genre_scores_gemma":[0.97312295,0.002557079,0.0052137906,0.00036059032,0.0005060209,0.000048560156,0.00049711706,0.000095493444,0.017598365],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99987376,0.000018398936,0.0000056720696,0.000040358686,0.00003333479,0.000028363214],"domain_scores_gemma":[0.99980384,0.00006816833,0.00004345926,0.0000354167,0.000017508943,0.000031530202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016396174,0.00038559813,0.0003262006,0.0003698108,0.00036040586,0.00089147326,0.00032001745,0.0005453564,0.0053688213],"category_scores_gemma":[0.00065655925,0.00015541182,0.00035673165,0.00026155563,0.0006392633,0.001058511,0.0008756529,0.0006193376,0.00074083876],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005207199,0.00017294567,0.014581559,0.0008725317,0.00024367233,0.0045383684,0.00067433156,0.055918455,0.02340463,0.7434593,0.021222176,0.1343914],"study_design_scores_gemma":[0.00021228414,0.00062643364,0.04246881,0.00025103037,0.00022046184,0.012838974,0.0008538196,0.097854614,0.017390838,0.5011988,0.32595894,0.00012493497],"about_ca_topic_score_codex":0.00024380752,"about_ca_topic_score_gemma":0.00013960159,"teacher_disagreement_score":0.0053688213,"about_ca_system_score_codex":0.00030860334,"about_ca_system_score_gemma":0.00012593316,"threshold_uncertainty_score":0.017960548},"labels":[],"label_agreement":null},{"id":"W2592600916","doi":"10.3847/1538-4357/aa7ed7","title":"Using Long-term Millisecond Pulsar Timing to Obtain Physical Characteristics of the Bulge Globular Cluster Terzan 5","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Millisecond pulsar; Pulsar; Bulge; Milky Way; RADIUS; Proper motion; Astronomy; Star cluster; Galaxy; Stars","score_opus":0.026946304259333295,"score_gpt":0.2798082747191056,"score_spread":0.25286197045977227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2592600916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990095,0.000044701897,0.00023258073,0.0000063080047,0.0000031660188,0.0000025156294,0.0001249088,0.000010037206,0.0005661541],"genre_scores_gemma":[0.9990206,0.000019449295,0.0003776653,0.0000039294596,0.000001787707,0.0000021149885,0.00039101648,0.0000025756192,0.00018086229],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999573,0.0000030821618,0.0000030828908,0.000013531116,0.0000099047875,0.00001309019],"domain_scores_gemma":[0.9996685,0.000046193276,0.00010702765,0.000032611093,0.00006734472,0.000078422745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017031874,0.0001598979,0.00011310078,0.0010017281,0.0002179763,0.0002972293,0.00025573687,0.00017580071,0.000709546],"category_scores_gemma":[0.00045909427,0.000073903095,0.00014438151,0.00046824213,0.00014583017,0.00020782325,0.00040447665,0.00014385903,0.0002504507],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001604436,0.00001718521,0.9692637,0.000011993401,0.000034550038,0.0001602954,0.00015120757,0.0012087564,0.02320689,0.00015730434,0.00016001986,0.0054676244],"study_design_scores_gemma":[0.0000026305718,0.000036916015,0.9956819,0.0000035520868,0.000006949636,0.00009395941,0.000120280034,0.0022933101,0.0014090855,0.000049728536,0.00029784616,0.0000039527426],"about_ca_topic_score_codex":0.0049338094,"about_ca_topic_score_gemma":0.007676626,"teacher_disagreement_score":0.0049338094,"about_ca_system_score_codex":0.00032433565,"about_ca_system_score_gemma":0.00007651967,"threshold_uncertainty_score":0.00981015},"labels":[],"label_agreement":null},{"id":"W2592660322","doi":"10.3847/1538-4357/aa5df0","title":"A Search for L/T Transition Dwarfs with Pan-STARRS1 and WISE. III. Young L Dwarf Discoveries and Proper Motion Catalogs in Taurus and Scorpius–Centaurus","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; University of California, Los Angeles; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Space Telescope Science Institute; Queen's University Belfast; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; California Institute of Technology; Queen's University; Johns Hopkins University; Durham University; Smithsonian Institution","keywords":"Pleiades; Brown dwarf; Photometry (optics); Stellar classification; Proper motion; Stars; Massive compact halo object","score_opus":0.013102676123380919,"score_gpt":0.2445731633741252,"score_spread":0.2314704872507443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2592660322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99890554,0.00007759884,0.00013823202,0.000013953777,0.0000019285958,0.00000697974,0.00024975173,0.000022862194,0.0005832481],"genre_scores_gemma":[0.99786395,0.000052250896,0.00058490643,0.000019297504,0.00000733476,0.00000617458,0.0011062154,0.0000058345954,0.00035406247],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982506,0.000012556822,0.000014297312,0.00005857679,0.0000476889,0.000041893854],"domain_scores_gemma":[0.99904805,0.000076375494,0.00040540812,0.00007804775,0.00010549211,0.00028659406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037253308,0.00019720364,0.00018901197,0.0021141276,0.00048043416,0.00045365855,0.00023701506,0.00018065012,0.0010102532],"category_scores_gemma":[0.0005285423,0.00013627003,0.00020064188,0.00087524834,0.00023380613,0.00028550514,0.0005983365,0.0001699283,0.00038878797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011736289,0.000028655963,0.9584301,0.00001959194,0.00001957498,0.0003030883,0.00027089438,0.000054609583,0.03122696,0.000047801066,0.00019363716,0.009287659],"study_design_scores_gemma":[0.0000031691354,0.000067071756,0.99634886,0.0000026062755,0.000010949873,0.0004167407,0.00014280599,0.0001672269,0.0021536704,0.000014567544,0.00067029655,0.000002155438],"about_ca_topic_score_codex":0.0022192693,"about_ca_topic_score_gemma":0.005401233,"teacher_disagreement_score":0.0022192693,"about_ca_system_score_codex":0.00018923558,"about_ca_system_score_gemma":0.00020031272,"threshold_uncertainty_score":0.0044127107},"labels":[],"label_agreement":null},{"id":"W2592867994","doi":"10.3847/1538-4357/aa6159","title":"The Secret Lives of Cepheids: δ Cep—The Prototype of a New Class of Pulsating X-Ray Variable Stars<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Cepheid variable; Variable star; Astrophysics; Stars; Astronomy; Class (philosophy); Artificial intelligence","score_opus":0.014926918116356228,"score_gpt":0.24113787047583246,"score_spread":0.22621095235947625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2592867994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9450925,0.0018500347,0.0036639285,0.0029762143,0.00047809083,0.00006615815,0.0035380481,0.00036944685,0.041965578],"genre_scores_gemma":[0.98911256,0.00045849854,0.0039461018,0.00044544094,0.00012234741,0.00002062965,0.0020153592,0.000053975073,0.0038250417],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985707,0.00001984515,0.000006524843,0.000035723726,0.00005632413,0.000024396571],"domain_scores_gemma":[0.9992555,0.00013587797,0.00016264526,0.00011969858,0.000113138056,0.00021318665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032399263,0.00017515018,0.00015165181,0.00034705864,0.00090513896,0.0011000722,0.00029654798,0.00025542348,0.0036405795],"category_scores_gemma":[0.00093901565,0.00009516821,0.00008412726,0.0005144687,0.00095843244,0.0007803515,0.0006609556,0.0006962038,0.00049731234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023334853,0.00022016624,0.45706436,0.00038497022,0.00007651094,0.0065197656,0.0050205416,0.000993654,0.03970304,0.07467372,0.12490933,0.2881005],"study_design_scores_gemma":[0.000062885854,0.0004216651,0.6265994,0.000109937,0.000045866946,0.0068730214,0.0040247464,0.0025252695,0.017077247,0.013500998,0.3286811,0.000077865756],"about_ca_topic_score_codex":0.0017685663,"about_ca_topic_score_gemma":0.0027484728,"teacher_disagreement_score":0.0036405795,"about_ca_system_score_codex":0.00040106082,"about_ca_system_score_gemma":0.00024126476,"threshold_uncertainty_score":0.012179017},"labels":[],"label_agreement":null},{"id":"W2593291216","doi":"10.3847/1538-4357/aa713f","title":"Limits on the Ultra-bright Fast Radio Burst Population from the CHIME Pathfinder","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; National Research Council Canada; Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; Dominion Astrophysical Observatory; Canadian Institute for Advanced Research; University of British Columbia","funders":"","keywords":"Fast radio burst; Pathfinder; Population; Brightness; Sky; Range (aeronautics); Flux (metallurgy); Magnetic field","score_opus":0.020812170017477073,"score_gpt":0.3041522810191789,"score_spread":0.2833401110017018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2593291216","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9859886,0.00032417398,0.004624751,0.00027227335,0.000010750879,0.00003827428,0.002515069,0.00018008788,0.0060461294],"genre_scores_gemma":[0.98905855,0.000091203954,0.005334252,0.000105870306,0.000012939098,0.00002824906,0.0039141597,0.000061091276,0.0013936843],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985227,0.00012353623,0.000021889322,0.0003259592,0.00070486835,0.0003010306],"domain_scores_gemma":[0.9962431,0.0007652192,0.0004532758,0.0005272945,0.0011909382,0.0008201591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001769486,0.00045176604,0.0004134479,0.0016705755,0.0008765674,0.00092627894,0.00095933315,0.00048106952,0.0017095227],"category_scores_gemma":[0.004503582,0.00032365115,0.00019818326,0.0010010274,0.0007669989,0.00042887204,0.0011290326,0.00043339943,0.0005175943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010179391,0.00007777996,0.8805208,0.00006756686,0.00017258443,0.00053462817,0.0010063773,0.0047199945,0.05132104,0.0019224446,0.006437737,0.05220115],"study_design_scores_gemma":[0.000044094893,0.000072006595,0.9690805,0.00002717017,0.000046519603,0.00035874566,0.00023095636,0.010788353,0.007200962,0.00063087925,0.01142385,0.000095944124],"about_ca_topic_score_codex":0.20486818,"about_ca_topic_score_gemma":0.31629196,"teacher_disagreement_score":0.20486818,"about_ca_system_score_codex":0.0021563792,"about_ca_system_score_gemma":0.0012481392,"threshold_uncertainty_score":0.40735143},"labels":[],"label_agreement":null},{"id":"W2593442493","doi":"10.3847/1538-4357/aa7569","title":"Extending the Search for Muon Neutrinos Coincident with Gamma-Ray Bursts in IceCube Data","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":183,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; University of Oxford; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Neutrino; Muon; Gamma-ray burst; Neutrino astronomy; Neutrino detector; Muon neutrino; Measurements of neutrino speed","score_opus":0.03791224617147059,"score_gpt":0.29984531826460015,"score_spread":0.26193307209312955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2593442493","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98922604,0.00020366917,0.001921847,0.000044546163,0.000016136353,0.000049550403,0.005216611,0.00010109834,0.0032205312],"genre_scores_gemma":[0.96825045,0.00032915847,0.009776147,0.000056140994,0.00003481933,0.00008501585,0.020799011,0.000056338748,0.00061285764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999539,0.000094832554,0.000031660435,0.00013680066,0.00010976122,0.00008794675],"domain_scores_gemma":[0.99853015,0.00051958405,0.00033544263,0.00026837122,0.0002010886,0.000145448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010871668,0.00035152168,0.00040862156,0.0017469225,0.00039522914,0.0010859257,0.00039036025,0.00023597556,0.0012169547],"category_scores_gemma":[0.0016343598,0.00016228377,0.00047672942,0.0016866592,0.00022134441,0.00042584134,0.0008429756,0.00026048726,0.00022350032],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010242561,0.00017507956,0.9271975,0.00010769883,0.00035596805,0.00057044526,0.00021014718,0.008431085,0.026182594,0.0011068219,0.0015782096,0.033060305],"study_design_scores_gemma":[0.00014121522,0.00029133115,0.90317535,0.00006283533,0.00025391678,0.0009434063,0.00040037205,0.03925179,0.0365842,0.0013659464,0.017488377,0.000041158848],"about_ca_topic_score_codex":0.008097364,"about_ca_topic_score_gemma":0.011506695,"teacher_disagreement_score":0.008097364,"about_ca_system_score_codex":0.0005222599,"about_ca_system_score_gemma":0.00064074976,"threshold_uncertainty_score":0.016100466},"labels":[],"label_agreement":null},{"id":"W2593807707","doi":"10.3847/1538-4357/837/1/32","title":"SDSS IV MaNGA: Discovery of an Hα Blob Associated with a Dry Galaxy Pair—Ejected Gas or a “Dark” Galaxy Candidate?","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Lawrence Berkeley National Laboratory; Japan Society for the Promotion of Science; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Ministério da Ciência, Tecnologia e Inovação; Centre National d’Etudes Spatiales; Carnegie Institution for Science; Centre National de la Recherche Scientifique; University of Oxford; York University; New Mexico State University; Associated Universities; U.S. Department of Energy; Smithsonian Institution; National Radio Astronomy Observatory; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Algorithm; Physics; Computer science","score_opus":0.008246631218735038,"score_gpt":0.2206022972577239,"score_spread":0.21235566603898887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2593807707","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946679,0.00028602002,0.00069865014,0.00027240915,0.000022386841,0.000016486241,0.00047433825,0.00015427475,0.003407629],"genre_scores_gemma":[0.99711335,0.00007126651,0.0011766733,0.0001512671,0.000029321083,0.000006742897,0.00055041537,0.00002563227,0.00087523315],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999274,0.000004886638,0.0000034472014,0.000024074561,0.000016702716,0.000023514025],"domain_scores_gemma":[0.9996331,0.000037762446,0.00010185054,0.00004214883,0.000027533695,0.00015762709],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020729742,0.00020959933,0.0001653285,0.00088797585,0.0005127208,0.00052991824,0.00027097293,0.00035369882,0.0020774573],"category_scores_gemma":[0.00030491228,0.00019639263,0.00013815696,0.0003405269,0.00040587914,0.00028737253,0.00059093535,0.00026274487,0.0008751183],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058454636,0.00009438438,0.81598175,0.00008342557,0.00007739164,0.011611775,0.00056751026,0.00020838331,0.15208478,0.00087965804,0.0039192676,0.013907126],"study_design_scores_gemma":[0.00002567266,0.0001318252,0.96489835,0.00003070225,0.000040450246,0.009942279,0.00043810596,0.001580124,0.011009331,0.00047547746,0.011407488,0.000020219964],"about_ca_topic_score_codex":0.0015840469,"about_ca_topic_score_gemma":0.002712348,"teacher_disagreement_score":0.0020774573,"about_ca_system_score_codex":0.00031268317,"about_ca_system_score_gemma":0.00009814843,"threshold_uncertainty_score":0.0069497824},"labels":[],"label_agreement":null},{"id":"W2594040717","doi":"10.3847/1538-4357/aadd47","title":"The 2.4 μm Galaxy Luminosity Function as Measured Using WISE. III. Measurement Results","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Portsmouth; University of California, Los Angeles; York University; Space Telescope Science Institute; Science and Technology Facilities Council; Carnegie Mellon University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; Yale University; Vanderbilt University; National Science Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory","keywords":"Galaxy; Sky; Redshift; Luminosity; Luminosity function; Stellar mass; Infrared; Spectral energy distribution; Measure (data warehouse); Covariance","score_opus":0.024389528869460428,"score_gpt":0.23007043369158903,"score_spread":0.20568090482212859,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2594040717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96278,0.00012212114,0.009333246,0.00007229797,0.00001971441,0.000031604737,0.021780957,0.0012081892,0.0046518934],"genre_scores_gemma":[0.9721705,0.00003426603,0.0078345565,0.000054419772,0.00001569626,0.000067042165,0.018628513,0.00011857376,0.0010765347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995078,0.000084550884,0.000025090894,0.00013705129,0.00016842717,0.00007703807],"domain_scores_gemma":[0.99851936,0.0002189137,0.00041808255,0.0003553713,0.00037823417,0.00011001511],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008844268,0.0006221537,0.00042000832,0.002019576,0.00024621972,0.0006488922,0.0005133469,0.0004961634,0.0016565401],"category_scores_gemma":[0.0025903163,0.00024141364,0.0006162458,0.0015271789,0.00023164004,0.00060917344,0.0005577724,0.00039542138,0.0017935392],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027313837,0.000080414575,0.933542,0.00006229871,0.00016481693,0.00010667535,0.00013387529,0.007697106,0.024703834,0.0010152513,0.0039185802,0.028301917],"study_design_scores_gemma":[0.0000057851034,0.00006131421,0.97383094,0.0000063463776,0.000030321606,0.00016199499,0.00008338422,0.010120957,0.012920308,0.0002502506,0.002504144,0.00002427779],"about_ca_topic_score_codex":0.0037916626,"about_ca_topic_score_gemma":0.0038828182,"teacher_disagreement_score":0.0037916626,"about_ca_system_score_codex":0.0005069852,"about_ca_system_score_gemma":0.00014977728,"threshold_uncertainty_score":0.007539153},"labels":[],"label_agreement":null},{"id":"W2594159061","doi":"10.3847/1538-4357/aa6032","title":"Updated 34-band Photometry for the SINGS/KINGFISH Samples of Nearby Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Los Alamos National Laboratory; Science and Technology Facilities Council; National Aeronautics and Space Administration; California Institute of Technology; Eötvös Loránd Tudományegyetem; Max-Planck-Gesellschaft; Space Telescope Science Institute; Alfred P. Sloan Foundation; U.S. Department of Energy; National Science Foundation","keywords":"Photometry (optics); Astrophysics; Galaxy; Astronomy; Physics; Stars","score_opus":0.01646471181446681,"score_gpt":0.24725497147926417,"score_spread":0.23079025966479735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2594159061","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8151376,0.00081580126,0.0050353874,0.00021427812,0.00010278833,0.00017638346,0.16040005,0.0013337156,0.01678399],"genre_scores_gemma":[0.63217795,0.0005681039,0.023466382,0.0002453198,0.00013579472,0.0002800128,0.3320138,0.0005919821,0.010520674],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99878186,0.00007860638,0.00013055385,0.00032542003,0.00050513586,0.00017837397],"domain_scores_gemma":[0.99523735,0.00018360584,0.00094729883,0.0016859847,0.001416282,0.0005294185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010693958,0.0004249794,0.0005873006,0.007008689,0.0005501311,0.00088162464,0.000816181,0.00026593727,0.00809947],"category_scores_gemma":[0.0024876217,0.00040202565,0.00058522273,0.0042444724,0.00028139295,0.00092050084,0.002066532,0.0005167402,0.0045943432],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002898302,0.00008395001,0.8152942,0.0003032665,0.00018092437,0.00015495543,0.00077504903,0.0011133099,0.02691381,0.0009813076,0.042539988,0.111369364],"study_design_scores_gemma":[0.000011733196,0.00003342177,0.95361894,0.000029104538,0.00004193956,0.0001263035,0.00012732287,0.0003368857,0.0017850323,0.00017374748,0.04369783,0.000017822444],"about_ca_topic_score_codex":0.01608636,"about_ca_topic_score_gemma":0.032265082,"teacher_disagreement_score":0.01608636,"about_ca_system_score_codex":0.00082060596,"about_ca_system_score_gemma":0.0007720279,"threshold_uncertainty_score":0.03198546},"labels":[],"label_agreement":null},{"id":"W2594279543","doi":"10.3847/1538-4357/aa6305","title":"Imaging the Schwarzschild-radius-scale Structure of M87 with the Event Horizon Telescope Using Sparse Modeling","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":176,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astronomical interferometer; Interferometry; Iterative reconstruction; Astrophysics; Image resolution; Regularization (linguistics); Event horizon; Brightness; Optics; Algorithm; Event (particle physics); Computer science; Computer vision; Artificial intelligence","score_opus":0.014497351569053643,"score_gpt":0.24255254343368723,"score_spread":0.22805519186463358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2594279543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97743076,0.00006707942,0.021507103,0.00012895085,0.000003997228,0.000006395939,0.00009380013,0.00011614473,0.0006457973],"genre_scores_gemma":[0.99642026,0.000013779378,0.00340363,0.000010665358,0.0000044226267,0.0000023716834,0.00009540497,0.0000064256665,0.000043110376],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989784,0.000040408027,0.000003490844,0.000019575147,0.000020907408,0.000017884007],"domain_scores_gemma":[0.9996749,0.000098521195,0.00009114598,0.000061311686,0.000032441007,0.00004164261],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005599465,0.00029846423,0.00028117895,0.00034400536,0.0001892769,0.00037974713,0.00048170434,0.00030089592,0.00028981915],"category_scores_gemma":[0.0009621318,0.00016574268,0.00040282318,0.00031681938,0.0003660174,0.0003660191,0.00044807547,0.00030275626,0.00005930059],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029305025,0.00014743615,0.085108615,0.000053908487,0.00020720018,0.00037862392,0.0002541671,0.83569044,0.046985935,0.0065125166,0.0010346591,0.023333509],"study_design_scores_gemma":[0.00001836319,0.000029130599,0.036274068,0.0000028915385,0.000013451528,0.000030569656,0.00003089512,0.96098506,0.0013298509,0.0011239183,0.00014995683,0.000011788451],"about_ca_topic_score_codex":0.005758308,"about_ca_topic_score_gemma":0.0056657377,"teacher_disagreement_score":0.005758308,"about_ca_system_score_codex":0.00041779142,"about_ca_system_score_gemma":0.00034114136,"threshold_uncertainty_score":0.011449575},"labels":[],"label_agreement":null},{"id":"W2594778558","doi":"10.3847/1538-4357/aa7684","title":"Giant Primeval Magnetic Dipoles","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Astrophysics; Dark matter; Dipole; Quantum mechanics","score_opus":0.009284287407478269,"score_gpt":0.23282922902618336,"score_spread":0.22354494161870508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2594778558","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94493973,0.00054043176,0.0066148057,0.0005887349,0.000073768126,0.000020213334,0.00023411511,0.00029717496,0.046690904],"genre_scores_gemma":[0.9963862,0.00008104547,0.0005559573,0.000034003097,0.000017871287,0.000002621177,0.000058796584,0.000006232034,0.0028573724],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999733,0.0000032123244,5.1403316e-7,0.000009081482,0.0000050805443,0.000008808768],"domain_scores_gemma":[0.9998486,0.00003352885,0.000047094654,0.00002007598,0.000017282282,0.000033392687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007142658,0.00016908962,0.000089742905,0.00028642392,0.00033161262,0.00032784237,0.00015151376,0.00019036393,0.004191634],"category_scores_gemma":[0.00031261612,0.000059422415,0.00009243559,0.00018302299,0.00048146586,0.00020277513,0.00032834252,0.00023074595,0.0005068171],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008125946,0.0001075154,0.22121246,0.00040055637,0.00009568073,0.0058748494,0.002261368,0.008081702,0.12300753,0.45832446,0.022278408,0.15754288],"study_design_scores_gemma":[0.00019760104,0.0008521119,0.40319386,0.000098747776,0.00010852513,0.024768187,0.0016429195,0.023928251,0.052669592,0.21532087,0.27714077,0.00007851714],"about_ca_topic_score_codex":0.00035701576,"about_ca_topic_score_gemma":0.00031089463,"teacher_disagreement_score":0.004191634,"about_ca_system_score_codex":0.00030705376,"about_ca_system_score_gemma":0.000102829654,"threshold_uncertainty_score":0.01402241},"labels":[],"label_agreement":null},{"id":"W2594881261","doi":"10.1086/309067","title":"General Relativistic Cosmology with No Beginning of Time","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; General relativity; Cosmology; Gravitational singularity; Inflation (cosmology); Theoretical physics; Initial singularity; Singularity; Cosmological principle; Theory of relativity; Classical mechanics; Metric expansion of space; Universe; De Sitter universe; Dark energy; Astrophysics; Quantum mechanics","score_opus":0.004207079573755653,"score_gpt":0.2166259414495224,"score_spread":0.21241886187576675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2594881261","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.046265177,0.019988917,0.29490426,0.02610614,0.0029238549,0.000055466364,0.00024880382,0.00082664465,0.6086807],"genre_scores_gemma":[0.8154085,0.0074072205,0.09264653,0.0056272247,0.002307263,0.00010285859,0.00022260255,0.0002962145,0.07598159],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99941576,0.00018812565,0.000025197856,0.000121098936,0.00018757994,0.00006236065],"domain_scores_gemma":[0.9993919,0.00011492423,0.00006278559,0.00027939258,0.00008017238,0.00007080574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010425325,0.00053793896,0.0006373033,0.00066163024,0.0014051769,0.0025543591,0.00088393316,0.0013800643,0.0032663948],"category_scores_gemma":[0.0017075462,0.00029047084,0.00077213673,0.00046131556,0.010687928,0.006080997,0.0022409544,0.0034169606,0.0012336283],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000001838155,0.0000014530273,0.000029292494,0.000009285483,0.0000018029732,0.000017868784,0.0000828915,0.00008409124,0.000066706765,0.99811053,0.00049312203,0.0011011222],"study_design_scores_gemma":[0.0000046669616,0.000011304375,0.000058789097,0.000014561663,0.0000033437282,0.00007464184,0.000033624943,0.00031020519,0.00008721855,0.97337306,0.026022665,0.000005896245],"about_ca_topic_score_codex":0.0009261042,"about_ca_topic_score_gemma":0.0008954816,"teacher_disagreement_score":0.0032663948,"about_ca_system_score_codex":0.0012937068,"about_ca_system_score_gemma":0.0010277751,"threshold_uncertainty_score":0.0109272},"labels":[],"label_agreement":null},{"id":"W2595474171","doi":"10.3847/1538-4357/aa61a9","title":"NGC 3105: A Young Cluster in the Outer Galaxy<sup>∗</sup> <sup>†</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Stars; Photometry (optics); Open cluster; Blue straggler; Hertzsprung–Russell diagram; Star cluster; Spectral line; Luminosity; Cluster (spacecraft)","score_opus":0.01454461431026563,"score_gpt":0.24217115436911385,"score_spread":0.22762654005884822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2595474171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9771035,0.00035424109,0.00048947276,0.00017948967,0.00006261934,0.00002860404,0.0047948547,0.00011400541,0.016873125],"genre_scores_gemma":[0.986382,0.00009596789,0.00076811144,0.000058194695,0.000020367295,0.0000071789445,0.0050277244,0.00001035717,0.0076301903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993217,0.0000026551245,0.000005215842,0.0000181308,0.00002127196,0.000020594558],"domain_scores_gemma":[0.9998584,0.0000079046395,0.000023199063,0.0000063942202,0.000012628938,0.0000914723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008157633,0.00011125709,0.000092227005,0.0004294663,0.0006258401,0.00022344086,0.00024556305,0.00014625366,0.007879614],"category_scores_gemma":[0.0001534586,0.000051895473,0.000081232356,0.0004931843,0.00024828265,0.00018261823,0.00028063686,0.000086258304,0.002015582],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009978901,0.0001353023,0.82092404,0.00029832224,0.00004198066,0.005439317,0.0023051007,0.0011470228,0.050766125,0.0047209044,0.038109615,0.07511442],"study_design_scores_gemma":[0.0000043046766,0.00008213913,0.9762482,0.00001954601,0.000009243269,0.000904515,0.000571538,0.00023542109,0.00084905024,0.00019813274,0.020870661,0.0000073340198],"about_ca_topic_score_codex":0.026098927,"about_ca_topic_score_gemma":0.043107007,"teacher_disagreement_score":0.026098927,"about_ca_system_score_codex":0.00066658447,"about_ca_system_score_gemma":0.00032399912,"threshold_uncertainty_score":0.05189407},"labels":[],"label_agreement":null},{"id":"W2596629336","doi":"10.3847/1538-4357/aa662d","title":"IC 630: Piercing the Veil of the Nuclear Gas","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Cancer Institute; Australian Astronomical Optics-Macquarie; Science and Technology Facilities Council; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Ministerio de Ciencia, Tecnología e Innovación Productiva; Science Mission Directorate; Queen's University Belfast; Gordon and Betty Moore Foundation; Swinburne University of Technology; National Central University; Planetary Science Division; Monash University; Space Telescope Science Institute; National Computational Infrastructure; Los Alamos National Laboratory; Johns Hopkins University; Ministério da Ciência, Tecnologia e Inovação; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; Curtin University of Technology; California Institute of Technology; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Luminosity; Star formation; Galaxy; Stars; Excitation; Star cluster; Black hole (networking); Velocity dispersion; Astronomy","score_opus":0.008141032387195823,"score_gpt":0.21014105857474188,"score_spread":0.20200002618754606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2596629336","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99198115,0.00006548308,0.0007257858,0.000028563845,0.000007416225,0.000009644755,0.00025646537,0.00009775922,0.006827679],"genre_scores_gemma":[0.998836,0.000016695707,0.0004668709,0.000015777643,0.0000028540578,0.0000026831344,0.00016298807,0.000014502369,0.00048165562],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992526,0.0000034547734,0.0000022703634,0.000020202942,0.000023882947,0.000024993667],"domain_scores_gemma":[0.99976104,0.000013583558,0.000052755087,0.00002342498,0.00002833358,0.000120798715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007380611,0.00026260212,0.00018595393,0.00035849062,0.0003781426,0.00062917545,0.00028028258,0.00025273868,0.002142984],"category_scores_gemma":[0.00033547723,0.00011384326,0.000102065125,0.00032326847,0.0004138602,0.00023713033,0.0006778826,0.00026446747,0.00053835183],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008840761,0.00019491956,0.37303105,0.00009751775,0.0000595451,0.0051959543,0.0010486986,0.006585415,0.5647869,0.005330891,0.0037166656,0.03906842],"study_design_scores_gemma":[0.00003343667,0.00031578637,0.9411773,0.000031265594,0.000026007892,0.0021907715,0.00059193437,0.017174806,0.03138579,0.0015577482,0.0054887305,0.00002642489],"about_ca_topic_score_codex":0.011145285,"about_ca_topic_score_gemma":0.008270268,"teacher_disagreement_score":0.011145285,"about_ca_system_score_codex":0.0005022932,"about_ca_system_score_gemma":0.00027011812,"threshold_uncertainty_score":0.022160828},"labels":[],"label_agreement":null},{"id":"W2596708082","doi":"10.3847/1538-4357/aa662a","title":"SDSS-IV MaNGA: Variation of the Stellar Initial Mass Function in Spiral and Early-type Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Youth Innovation Promotion Association; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Ministry of Education, Culture, Sports, Science and Technology; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Galaxy; Spiral galaxy; Initial mass function; Elliptical galaxy; Stellar population; Stellar mass; RADIUS; Bulge; Variation (astronomy)","score_opus":0.010932864353983668,"score_gpt":0.22152360017850603,"score_spread":0.21059073582452237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2596708082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99897873,0.000048154874,0.00026394334,0.00002585879,0.0000017564716,0.0000022840732,0.00033150488,0.00006348653,0.00028426485],"genre_scores_gemma":[0.9988457,0.000013300093,0.0003156989,0.0000072895245,0.000002784798,0.000003377185,0.0006755414,0.000029995785,0.000106346524],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979144,0.00006572561,0.0000108889735,0.00006467289,0.000023049031,0.000044282828],"domain_scores_gemma":[0.9991586,0.00024284008,0.00018176783,0.0001402133,0.00009225805,0.00018430428],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010076785,0.00031838057,0.00031681967,0.0009372012,0.00030805156,0.0005591148,0.00032046047,0.00023812996,0.00058122794],"category_scores_gemma":[0.0012275313,0.00018595924,0.00054893264,0.00053586916,0.000276599,0.00023935527,0.0003922803,0.00022497811,0.00031711732],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014929492,0.000034012144,0.9777761,0.00001780834,0.00010182602,0.00006791069,0.00020489814,0.011243941,0.006754534,0.00037834366,0.0003996431,0.0028716447],"study_design_scores_gemma":[0.000013655005,0.00002429122,0.95504725,0.0000066413063,0.000025624096,0.000038747577,0.00011408527,0.042951338,0.001149339,0.00013504425,0.0004827347,0.000011227064],"about_ca_topic_score_codex":0.01310524,"about_ca_topic_score_gemma":0.011839022,"teacher_disagreement_score":0.01310524,"about_ca_system_score_codex":0.0006107198,"about_ca_system_score_gemma":0.000258062,"threshold_uncertainty_score":0.026057899},"labels":[],"label_agreement":null},{"id":"W2596716325","doi":"10.1088/0004-637x/716/1/712","title":"SPECTRA AND<i>HUBBLE SPACE TELESCOPE</i>LIGHT CURVES OF SIX TYPE Ia SUPERNOVAE AT 0.511 &lt;<i>z</i>&lt; 1.12 AND THE UNION2 COMPILATION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1350,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; Stockholms Universitet; Space Telescope Science Institute; Japan Society for the Promotion of Science; Office of Science; Drexel University; National Aeronautics and Space Administration; High Energy Physics; U.S. Department of Energy","keywords":"Physics; Astrophysics; Redshift; Light curve; Supernova; Photometry (optics); Hubble's law; Hubble space telescope; Astronomy; Type (biology); Cosmology; Spectral line; Galaxy; Stars","score_opus":0.0069558506723204514,"score_gpt":0.21877800400130815,"score_spread":0.21182215332898768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2596716325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.74239767,0.0008754374,0.0061252946,0.00010331013,0.000093636496,0.00014537711,0.21560286,0.0031839246,0.03147254],"genre_scores_gemma":[0.55500543,0.00055423967,0.016137082,0.00015037053,0.00014737745,0.00022385622,0.41759887,0.0014770384,0.008705697],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99914527,0.00012592514,0.00009778436,0.00012880078,0.00036044096,0.00014179562],"domain_scores_gemma":[0.99544513,0.00066053827,0.0011422572,0.0010993601,0.0012464797,0.00040621063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014220157,0.0009894709,0.00048040642,0.010381028,0.000772405,0.0011733985,0.00069359125,0.00042959693,0.0072389017],"category_scores_gemma":[0.002747622,0.0005326645,0.0007883647,0.005117954,0.00030142482,0.00068647653,0.001202552,0.00043890977,0.0028891498],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002575901,0.0004444851,0.75829905,0.00083406206,0.00058053003,0.0008874366,0.0014551191,0.00810335,0.018716114,0.0021113807,0.076533,0.12945955],"study_design_scores_gemma":[0.00002739703,0.00010390102,0.95866114,0.000036281843,0.00005131528,0.0004545855,0.00011864624,0.0017468398,0.0030132197,0.00021859708,0.035535943,0.000032319727],"about_ca_topic_score_codex":0.011181362,"about_ca_topic_score_gemma":0.021052834,"teacher_disagreement_score":0.011181362,"about_ca_system_score_codex":0.0006719637,"about_ca_system_score_gemma":0.0003602899,"threshold_uncertainty_score":0.024216533},"labels":[],"label_agreement":null},{"id":"W2596761680","doi":"10.3847/1538-4357/ab737e","title":"Constraints on the Intergalactic Magnetic Field from Bow Ties in the Gamma-Ray Sky","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Intergalactic travel; Cosmic microwave background; Halo; Blazar; Cosmic infrared background; Magnetic field; Sky; Anisotropy; Galactic halo","score_opus":0.012452023713135066,"score_gpt":0.2116689850793566,"score_spread":0.19921696136622155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2596761680","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948949,0.00011115536,0.0011011934,0.0000288991,0.0000031068662,0.0000019431666,0.00008945676,0.000011624495,0.003757697],"genre_scores_gemma":[0.9993352,0.000043432963,0.00033422638,0.0000136672315,0.0000075826238,0.0000012582267,0.00015276716,0.0000038139606,0.00010787328],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998292,0.000042602733,0.000011504465,0.0000368336,0.000047379657,0.00003234906],"domain_scores_gemma":[0.99789727,0.0010744418,0.00043101652,0.00020122771,0.00016168793,0.00023444109],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044897784,0.00034240147,0.00017558796,0.0010288331,0.00022652937,0.0009366393,0.00029221212,0.00031039855,0.0020920706],"category_scores_gemma":[0.0022811682,0.00019030007,0.00016477547,0.00052518793,0.0005644753,0.00060800265,0.00063886406,0.00029055754,0.00024850407],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080888945,0.000073169576,0.8510573,0.00012084775,0.00017809523,0.0004828819,0.00027454464,0.004833542,0.10734123,0.0103681665,0.000466507,0.023994831],"study_design_scores_gemma":[0.000045546785,0.000084507425,0.9745967,0.00003259257,0.0000901768,0.00025134248,0.00020102013,0.007362926,0.010669376,0.0055973255,0.0010495841,0.000018988247],"about_ca_topic_score_codex":0.0010786508,"about_ca_topic_score_gemma":0.0026481913,"teacher_disagreement_score":0.0020920706,"about_ca_system_score_codex":0.00017291911,"about_ca_system_score_gemma":0.00010904624,"threshold_uncertainty_score":0.006998658},"labels":[],"label_agreement":null},{"id":"W2596887988","doi":"10.3847/1538-4357/aa7512","title":"The Peculiar Multiwavelength Evolution Of V1535 Sco","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Synchrotron; Spectral energy distribution; Spectral line; Light curve; Thermal emission; Synchrotron radiation; Outflow; Emission spectrum; Shock (circulatory)","score_opus":0.01297978629746339,"score_gpt":0.24716855262366855,"score_spread":0.23418876632620517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2596887988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976871,0.00016308979,0.0001290139,0.00002349027,0.00000966975,0.000004973087,0.0001773574,0.000018070763,0.0017871973],"genre_scores_gemma":[0.9993179,0.000030063304,0.00012601516,0.000017735201,0.0000061471806,0.0000024362923,0.00028100426,0.000004860901,0.00021381713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999231,0.000004137389,0.000005900167,0.000024418643,0.000021381433,0.000021209094],"domain_scores_gemma":[0.9996574,0.000022630538,0.00012047466,0.00003128365,0.000046126337,0.00012208988],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014773813,0.0002120321,0.00021711507,0.00087711634,0.00049347914,0.0005248952,0.00023098919,0.00025428704,0.00063519424],"category_scores_gemma":[0.00038359224,0.00013794318,0.00022311493,0.00040354923,0.00025261147,0.00019476764,0.0005095986,0.00029411807,0.00017850484],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028487656,0.00008913017,0.8191449,0.00008485505,0.00016841952,0.0036447565,0.00066500733,0.000734132,0.15894578,0.00041367608,0.0010035108,0.014820974],"study_design_scores_gemma":[0.0000019479114,0.000030474677,0.99748504,0.000009644642,0.000008728668,0.00043727024,0.00007930149,0.00022760955,0.0009727904,0.000039511775,0.0007032903,0.0000042970464],"about_ca_topic_score_codex":0.0051211435,"about_ca_topic_score_gemma":0.0112430295,"teacher_disagreement_score":0.0051211435,"about_ca_system_score_codex":0.00049672625,"about_ca_system_score_gemma":0.00012368956,"threshold_uncertainty_score":0.010182679},"labels":[],"label_agreement":null},{"id":"W2596914018","doi":"10.1086/510342","title":"The Transit Light Curve Project. IV. Five Transits of the Exoplanet OGLE‐TR‐10b","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Exoplanet; Photometry (optics); Light curve; Ephemeris; Physics; Planet; Transit (satellite); Astronomy; RADIUS; Planetary system; Astrophysics; Stars","score_opus":0.009181408365506896,"score_gpt":0.22362458978535915,"score_spread":0.21444318141985225,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2596914018","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.66421485,0.0007670043,0.0074023926,0.0003963003,0.00013941039,0.0005691967,0.27269164,0.003025671,0.050793435],"genre_scores_gemma":[0.48014778,0.00033760595,0.031406086,0.00019896614,0.00008938146,0.00044285893,0.46786398,0.0008292423,0.018684013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997074,0.00004285134,0.000021635346,0.000092785776,0.00007639909,0.000058910824],"domain_scores_gemma":[0.9989374,0.000050202132,0.00024442162,0.00022433474,0.0002982179,0.00024542576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006991489,0.00057071645,0.00025091248,0.0025282286,0.00051059166,0.0006076064,0.0004159305,0.00033386168,0.005428261],"category_scores_gemma":[0.00072439143,0.0002492059,0.0002636764,0.0019249319,0.00014251785,0.00040218642,0.0009162482,0.0004029747,0.0038553653],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019811494,0.00080037955,0.5954078,0.00046783604,0.0002570186,0.0003798633,0.0012023696,0.0014963987,0.04081459,0.002292117,0.13488306,0.22001743],"study_design_scores_gemma":[0.000095098185,0.00023414652,0.888432,0.000027932163,0.00003641603,0.000269261,0.00014527596,0.0013282095,0.0045015574,0.0002592683,0.10465125,0.000019528787],"about_ca_topic_score_codex":0.019399635,"about_ca_topic_score_gemma":0.03811396,"teacher_disagreement_score":0.019399635,"about_ca_system_score_codex":0.0006781433,"about_ca_system_score_gemma":0.0005866966,"threshold_uncertainty_score":0.038573444},"labels":[],"label_agreement":null},{"id":"W2598284352","doi":"10.3847/1538-4357/aa64db","title":"Erratum: “Bayesian Mass Estimates of the Milky Way: Including Measurement Uncertainties with Hierarchical Bayes” (2017, ApJ, 835, 167)","year":2017,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; McMaster University","funders":"","keywords":"Physics; Milky Way; Bayes' theorem; Bayesian probability; Astrophysics; Statistics; Stars; Mathematics","score_opus":0.0271214573082583,"score_gpt":0.24897994811393656,"score_spread":0.22185849080567827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2598284352","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00038401235,0.0010985908,0.001649442,0.07535869,0.9072759,0.000028359074,0.0044536144,0.0007096594,0.009041796],"genre_scores_gemma":[0.022591487,0.0069834567,0.01334397,0.14746425,0.3455931,0.00028677998,0.019316185,0.005875601,0.43854523],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.997299,0.00039947574,0.0005054212,0.00040688837,0.0012318091,0.00015745398],"domain_scores_gemma":[0.9813679,0.0045825094,0.0010153998,0.0014378631,0.0109481355,0.00064817886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003057686,0.0018775889,0.0013110914,0.002798448,0.0034930513,0.004080947,0.0027602331,0.004449748,0.059649896],"category_scores_gemma":[0.053458147,0.0010002642,0.0011482505,0.0023159876,0.001829967,0.0039748494,0.0023553441,0.008140525,0.046430998],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00001620098,0.0000034452455,0.00006782189,0.00002389361,0.000004818688,0.000048226942,0.000010565308,0.000046085006,0.000025002779,0.00086154434,0.9964954,0.0023969943],"study_design_scores_gemma":[0.00005021482,0.000019485306,0.001534726,0.00029034642,0.000033500753,0.00024893,0.00012822912,0.00071793067,0.0005508801,0.008807822,0.9875471,0.00007074371],"about_ca_topic_score_codex":0.02764122,"about_ca_topic_score_gemma":0.032336857,"teacher_disagreement_score":0.059649896,"about_ca_system_score_codex":0.0037329525,"about_ca_system_score_gemma":0.005141433,"threshold_uncertainty_score":0.19954878},"labels":[],"label_agreement":null},{"id":"W2598332543","doi":"10.3847/1538-4357/aa6479","title":"Star Streams and the Assembly History of the Galaxy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Halo; Milky Way; Star cluster; Astronomy; Galactic halo; Galaxy; Velocity dispersion; Cluster (spacecraft); Population; Sky","score_opus":0.008463460816457226,"score_gpt":0.2045621722858906,"score_spread":0.1960987114694334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2598332543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976718,0.0001770821,0.00031651318,0.000026496797,0.000001996265,0.0000027470014,0.00025200262,0.000017213271,0.0015340861],"genre_scores_gemma":[0.9991592,0.0000578952,0.0001102817,0.000002582022,0.0000034088998,0.0000012970191,0.00030163216,0.000004939575,0.0003587998],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992085,0.000021593642,0.0000055879113,0.000025028572,0.000012578246,0.000014326295],"domain_scores_gemma":[0.99826235,0.0004810926,0.0006512125,0.00014145538,0.0001748526,0.00028914554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038689587,0.00011598468,0.00009635236,0.00087962806,0.0002920495,0.00086318044,0.00014890479,0.00018755262,0.001977072],"category_scores_gemma":[0.002229428,0.00016317194,0.00016324446,0.00048577035,0.00031198878,0.00041295477,0.00037169128,0.00017792963,0.0004232829],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000110273715,0.000022986203,0.9799759,0.00002159502,0.000056576504,0.00012730698,0.00026382896,0.00456862,0.0047160448,0.0024404589,0.00025667588,0.0074397856],"study_design_scores_gemma":[0.0000035189178,0.00003799105,0.9929987,0.000004157702,0.00001511844,0.000071865135,0.00007910369,0.0046118665,0.00053191744,0.0009501989,0.000690103,0.000005390872],"about_ca_topic_score_codex":0.003296852,"about_ca_topic_score_gemma":0.0032864425,"teacher_disagreement_score":0.003296852,"about_ca_system_score_codex":0.0004259455,"about_ca_system_score_gemma":0.00012829952,"threshold_uncertainty_score":0.0066140294},"labels":[],"label_agreement":null},{"id":"W2599048417","doi":"10.1086/513501","title":"Automatic Detection of Expanding H<scp>i</scp>Shells in the Canadian Galactic Plane Survey Data","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université Laval","funders":"","keywords":"Galactic plane; Pixel; Scale (ratio); Identification (biology); Plane (geometry); Signature (topology); Field (mathematics); Cardinal point","score_opus":0.037321553325098115,"score_gpt":0.30692418356037104,"score_spread":0.2696026302352729,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2599048417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98360854,0.00025178236,0.0041465005,0.0001267457,0.000009052938,0.00006237271,0.005061217,0.00047808746,0.0062558246],"genre_scores_gemma":[0.986326,0.00012191118,0.0076936507,0.000016293765,0.0000034676343,0.000012255318,0.0044743842,0.000026220812,0.001325784],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973994,0.000019479008,0.000009345649,0.000041955616,0.00012746784,0.000061798346],"domain_scores_gemma":[0.9993913,0.00006433934,0.00007626131,0.000037749207,0.0003457153,0.000084593456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003297658,0.00024317813,0.00015711205,0.0021960938,0.0006152443,0.00048475433,0.000384393,0.00013455762,0.0011038834],"category_scores_gemma":[0.0011748676,0.00012207736,0.00013944767,0.0014454473,0.00023321432,0.00017805166,0.0003234266,0.00014071152,0.00022828586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003938429,0.00006248266,0.74887806,0.0001874073,0.00011428786,0.00042839377,0.0006046704,0.0098490175,0.05960227,0.0017914545,0.011645689,0.16644241],"study_design_scores_gemma":[0.000014559314,0.000017598955,0.96526486,0.000011015771,0.000023611105,0.00008111748,0.00020561383,0.019595886,0.009322206,0.00009511128,0.005347419,0.000020958056],"about_ca_topic_score_codex":0.844216,"about_ca_topic_score_gemma":0.9234911,"teacher_disagreement_score":0.15578401,"about_ca_system_score_codex":0.0025512292,"about_ca_system_score_gemma":0.0027828868,"threshold_uncertainty_score":0.3134029},"labels":[],"label_agreement":null},{"id":"W2601882356","doi":"10.3847/1538-4357/aa6347","title":"The 2014 X-Ray Minimum of η Carinae as Seen by Swift","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Swift; X-ray; Telescope; Light curve; Line (geometry); Astronomy; X-ray telescope; X-ray binary; Neutron star; Geometry; Optics","score_opus":0.009272569516248386,"score_gpt":0.24528213305748864,"score_spread":0.23600956354124025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2601882356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983438,0.00008647577,0.00011820637,0.000020431426,0.000006070168,0.0000035737194,0.00014306573,0.000010430755,0.0012679516],"genre_scores_gemma":[0.9989273,0.000040273022,0.00013197828,0.000012702875,0.000014131715,0.000003682578,0.00046010411,0.000005422737,0.00040439982],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989617,0.000006501754,0.000006616643,0.000027750912,0.000037382557,0.000025469943],"domain_scores_gemma":[0.99973685,0.000017034068,0.00011336876,0.000020795893,0.000053660755,0.00005832886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018758194,0.00018210197,0.00024481636,0.00057353213,0.0004735935,0.0005208627,0.00021234444,0.00025151655,0.0007141689],"category_scores_gemma":[0.000422667,0.00014427252,0.00016850232,0.00032752464,0.00025462086,0.0002582146,0.0005982749,0.00027697533,0.00024629038],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065421476,0.0001092274,0.89821553,0.000059956277,0.00011562067,0.0011869408,0.0006903479,0.0008073622,0.081386425,0.0003359399,0.0012192898,0.015219234],"study_design_scores_gemma":[0.0000040233713,0.000059022113,0.9969958,0.000004074534,0.000008168431,0.00018243065,0.00007379305,0.00021568751,0.0012087579,0.000026142892,0.0012184207,0.000003665191],"about_ca_topic_score_codex":0.0026978347,"about_ca_topic_score_gemma":0.006076356,"teacher_disagreement_score":0.0026978347,"about_ca_system_score_codex":0.0002828408,"about_ca_system_score_gemma":0.00015632332,"threshold_uncertainty_score":0.005364239},"labels":[],"label_agreement":null},{"id":"W2602055580","doi":"10.1088/0004-637x/691/2/1634","title":"NON-LTE MODELING OF THE NEAR-ULTRAVIOLET BAND OF LATE-TYPE STARS","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Extinction (optical mineralogy); Stars; Flux (metallurgy); Physics; Astrophysics; Ultraviolet; Irradiance; Line (geometry); Spectral line; Molar absorptivity; Astronomy; Optics; Chemistry","score_opus":0.010658634119015771,"score_gpt":0.22306066010276704,"score_spread":0.21240202598375127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2602055580","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9763007,0.00012532684,0.021120017,0.00013247065,0.000010007647,0.0000119489705,0.00018276086,0.00010950054,0.0020072123],"genre_scores_gemma":[0.99725074,0.00004076542,0.0018033651,0.000031149102,0.0000074706886,0.000009466695,0.00016074398,0.0000240185,0.00067210145],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998155,0.00006037872,0.000010632727,0.000043962616,0.000029828012,0.000039777682],"domain_scores_gemma":[0.9984143,0.00089165353,0.00024185563,0.000110206725,0.0002146383,0.00012738213],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006970772,0.0004752133,0.0003577399,0.00037551072,0.00046221213,0.00084805366,0.0010683108,0.0007134808,0.0006393288],"category_scores_gemma":[0.0032982815,0.0002920559,0.0006285404,0.00028938786,0.00033062173,0.0009386489,0.0003658487,0.00038408092,0.00023519681],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000107256754,0.000054562817,0.050693445,0.000019368059,0.0000609948,0.00009685793,0.00008618684,0.9418455,0.001915002,0.001691174,0.0001621199,0.0032675671],"study_design_scores_gemma":[0.000008110722,0.000021289658,0.00640186,0.000002386725,0.000008276498,0.000025123487,0.000018983943,0.9921639,0.00038336794,0.00083566253,0.0001254752,0.000005586845],"about_ca_topic_score_codex":0.02620592,"about_ca_topic_score_gemma":0.01689214,"teacher_disagreement_score":0.02620592,"about_ca_system_score_codex":0.001000615,"about_ca_system_score_gemma":0.0005210395,"threshold_uncertainty_score":0.052106798},"labels":[],"label_agreement":null},{"id":"W2602810741","doi":"10.3847/1538-4357/aa63f8","title":"ALMA Observations of Starless Core Substructure in Ophiuchus","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Substructure; Astrophysics; Physics; Protostar; Star formation; Core (optical fiber); Fragmentation (computing); Astronomy; Molecular cloud; Stars; Computer science","score_opus":0.03851686027974427,"score_gpt":0.2791429211092257,"score_spread":0.2406260608294814,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2602810741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953246,0.000019100728,0.000057890433,0.0000043399773,6.6385815e-7,0.0000019020572,0.00008759537,0.000006818444,0.0002892088],"genre_scores_gemma":[0.99968517,0.0000058822357,0.000114585266,0.0000027001174,0.0000013479726,0.0000013357056,0.000110619374,8.029837e-7,0.00007758708],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999954,0.000004846298,0.0000028074687,0.000014531402,0.000011502193,0.000012287418],"domain_scores_gemma":[0.9998267,0.000023225864,0.000057349156,0.000018021237,0.000019233154,0.000055495035],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010485278,0.000083051586,0.00009820854,0.0008361724,0.0003065799,0.0002415753,0.0001537272,0.00013545658,0.000593239],"category_scores_gemma":[0.0003046708,0.00007935962,0.00007756865,0.0002868136,0.00015847867,0.00017378789,0.00025895695,0.000104251594,0.00007634722],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023413223,0.000058351252,0.91306555,0.000015610907,0.000027484748,0.0002112082,0.0002807195,0.0007839393,0.07725714,0.00029443094,0.00020364026,0.0075677778],"study_design_scores_gemma":[0.000008839822,0.00003974604,0.9963922,0.0000018976499,0.0000053826593,0.00006617687,0.000047180103,0.001406195,0.0016403634,0.00006840048,0.00032129715,0.0000023320845],"about_ca_topic_score_codex":0.0072079557,"about_ca_topic_score_gemma":0.013711585,"teacher_disagreement_score":0.0072079557,"about_ca_system_score_codex":0.00035075212,"about_ca_system_score_gemma":0.00011465926,"threshold_uncertainty_score":0.014331996},"labels":[],"label_agreement":null},{"id":"W2603828070","doi":"10.1086/375683","title":"A Major Soft Gamma Repeater-like Outburst and Rotation Glitch in the No-longer-so-anomalous X-Ray Pulsar 1E 2259+586","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":264,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Research Canada","funders":"","keywords":"Astrophysics; Pulsar; Physics; Glitch; Magnetar; Telescope; Amplitude; Gamma ray; Flux (metallurgy); Astronomy; Optics; Materials science","score_opus":0.00928907903724675,"score_gpt":0.278699939756289,"score_spread":0.26941086071904224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2603828070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994491,0.000052795993,0.00009746408,0.000014694891,0.0000054945526,0.000004771415,0.000056382763,0.0000150237565,0.00030430217],"genre_scores_gemma":[0.99912924,0.000057835023,0.00021055802,0.00003087825,0.000013029799,0.0000053119315,0.0002468723,0.000005433841,0.0003008245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993014,0.00000583326,0.0000065773893,0.000022517817,0.000019068751,0.000015874919],"domain_scores_gemma":[0.999686,0.00002284493,0.000116047224,0.000046472243,0.000024403518,0.00010422704],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011960736,0.00022494873,0.00031570377,0.00032230496,0.00035790194,0.0003395307,0.00024422022,0.00029625776,0.0005467651],"category_scores_gemma":[0.00032892934,0.00014569172,0.0002582732,0.00017224097,0.00023366125,0.00015034045,0.0005929871,0.0004827425,0.0001866946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015393682,0.00029049045,0.5747065,0.0001181079,0.00013666788,0.010497524,0.0011105549,0.00038978123,0.38567916,0.0002787884,0.00062923186,0.024623875],"study_design_scores_gemma":[0.000016668262,0.00047013783,0.9891121,0.0000069415564,0.00002055078,0.0040527177,0.00012425637,0.00028091666,0.005010836,0.000048361282,0.00084730075,0.000009213633],"about_ca_topic_score_codex":0.00087281194,"about_ca_topic_score_gemma":0.0020004183,"teacher_disagreement_score":0.00087281194,"about_ca_system_score_codex":0.00012959189,"about_ca_system_score_gemma":0.000056500787,"threshold_uncertainty_score":0.0018290877},"labels":[],"label_agreement":null},{"id":"W2604157616","doi":"10.3847/1538-4357/aa65cd","title":"A Hubble Space Telescope Survey for Novae in M87. II. Snuffing out the Maximum Magnitude–Rate of Decline Relation for Novae as a Non-standard Candle, and a Prediction of the Existence of Ultrafast Novae<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Space Telescope Science Institute; American Museum of Natural History; National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; Nova (rocket); Galaxy; Cosmic distance ladder; Astronomy; Hubble space telescope; White dwarf; Spiral galaxy; Magnitude (astronomy); Stars; Redshift","score_opus":0.029350932608933643,"score_gpt":0.2727955157885575,"score_spread":0.24344458317962384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2604157616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993915,0.00027453652,0.00019650033,0.00009104459,0.0000048983634,0.000013861653,0.003883652,0.00003367503,0.0015868171],"genre_scores_gemma":[0.9950736,0.00013283135,0.00039913837,0.000028467872,0.0000086186055,0.000011082266,0.0039556986,0.000005737359,0.00038472057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998715,0.000019619769,0.000007768132,0.000026222597,0.000039869043,0.00003510471],"domain_scores_gemma":[0.9990926,0.00013550968,0.00029895536,0.00008921656,0.0001169116,0.00026674956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003783058,0.00019914951,0.00018968323,0.0017008286,0.000306944,0.00031952848,0.0003006562,0.00033330166,0.0014800162],"category_scores_gemma":[0.0007588993,0.000106991174,0.0002649707,0.00096903293,0.00016186081,0.00024107896,0.00037449293,0.00023179335,0.0007015179],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037593145,0.000027265192,0.9931793,0.000013675339,0.00002794895,0.0001001726,0.00008611469,0.0004476355,0.0013273949,0.00012966177,0.0007892677,0.0038340439],"study_design_scores_gemma":[0.0000011312345,0.000006214757,0.9991904,0.000001835135,0.0000035264356,0.00002768635,0.000026596466,0.0004892497,0.00005613513,0.000017391345,0.00017908915,7.8852634e-7],"about_ca_topic_score_codex":0.01800478,"about_ca_topic_score_gemma":0.034712426,"teacher_disagreement_score":0.01800478,"about_ca_system_score_codex":0.00046553157,"about_ca_system_score_gemma":0.00022594933,"threshold_uncertainty_score":0.03579998},"labels":[],"label_agreement":null},{"id":"W2604447909","doi":"10.3847/1538-4357/aa6af3","title":"On the Origin of Sub-subgiant Stars. I. Demographics","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; McGill University; University of Manitoba","funders":"","keywords":"Subgiant; Blue straggler; Stars; Demographics; Open cluster; Globular cluster; Stellar evolution; Binary star; Red giant","score_opus":0.019052603800302038,"score_gpt":0.24554805469912042,"score_spread":0.22649545089881837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2604447909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96664244,0.0012217984,0.00050103874,0.0005409155,0.000033769695,0.0001791511,0.018755386,0.000044347154,0.01208107],"genre_scores_gemma":[0.977187,0.0010321104,0.00026433155,0.00042243948,0.000038709255,0.00023530277,0.01047447,0.000031482985,0.010314085],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960655,0.000039176666,0.000033263837,0.000118840755,0.000080015416,0.00012228524],"domain_scores_gemma":[0.9989077,0.00010214701,0.00039337884,0.00006727205,0.0002000256,0.00032938382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032147637,0.00015774582,0.00024286602,0.0018598045,0.00078981667,0.0005695329,0.00035855864,0.0002405963,0.011922849],"category_scores_gemma":[0.0014242417,0.00012242683,0.000101230275,0.0017414205,0.0002752248,0.0007932811,0.000813779,0.0003701039,0.0061167656],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059459882,0.000027762178,0.98362434,0.000043501528,0.0000048062316,0.00020640616,0.0011409108,0.000020671552,0.00061954657,0.00046487738,0.0030950622,0.010692598],"study_design_scores_gemma":[0.0000019660076,0.000047387242,0.988241,0.000019690951,0.0000027975955,0.0003902769,0.0008929272,0.000032255102,0.00011689005,0.000117651,0.0101345405,0.0000024797405],"about_ca_topic_score_codex":0.006132989,"about_ca_topic_score_gemma":0.0067704213,"teacher_disagreement_score":0.011922849,"about_ca_system_score_codex":0.00035164235,"about_ca_system_score_gemma":0.00043450808,"threshold_uncertainty_score":0.03988588},"labels":[],"label_agreement":null},{"id":"W2604655066","doi":"10.3847/1538-4357/aa6a59","title":"Detection of the Stellar Intracluster Medium in Perseus (Abell 426)","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Astronomy; Hubble sequence; Galaxy; Photometry (optics); Metallicity; Hubble space telescope; Stellar population; Star cluster; Elliptical galaxy; Star formation; Stars","score_opus":0.007194830565321268,"score_gpt":0.21054792737695946,"score_spread":0.20335309681163818,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2604655066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99781704,0.00013860081,0.00010736073,0.000015316076,0.0000043238856,0.0000035297865,0.00038113442,0.000025488373,0.0015072391],"genre_scores_gemma":[0.99863595,0.00005578802,0.00028825525,0.0000147252,0.0000051656557,0.0000022183124,0.0005224805,0.000004140079,0.00047132978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999948,0.000003023638,0.0000019749898,0.000020799234,0.000013223848,0.000012946291],"domain_scores_gemma":[0.99985933,0.000010472484,0.000034698016,0.0000120720815,0.000021845375,0.000061663544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008234154,0.00024372709,0.00012595717,0.0011913185,0.00033276097,0.00035595286,0.00016016464,0.00017624683,0.0014414974],"category_scores_gemma":[0.00012975697,0.00009580833,0.00008285446,0.00043848445,0.00021381372,0.0001508672,0.00040317743,0.000115248564,0.00045429383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023635336,0.000048067446,0.70438755,0.00005128556,0.000044188364,0.0013203254,0.0005322284,0.00015710182,0.27825826,0.0002988418,0.0005873442,0.014078543],"study_design_scores_gemma":[0.000004779974,0.00005053054,0.9906185,0.0000033967933,0.000008465215,0.0005798189,0.00019289336,0.00012446876,0.006775296,0.000060593404,0.0015779957,0.0000032370324],"about_ca_topic_score_codex":0.0053628962,"about_ca_topic_score_gemma":0.0073381076,"teacher_disagreement_score":0.0053628962,"about_ca_system_score_codex":0.0002219228,"about_ca_system_score_gemma":0.0000803871,"threshold_uncertainty_score":0.01066339},"labels":[],"label_agreement":null},{"id":"W2604995907","doi":"10.3847/1538-4357/aa72ef","title":"On the Origin of Sub-subgiant Stars. III. Formation Frequencies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Subgiant; Globular cluster; Blue straggler; Stars; Stellar collision; Red giant; Stellar evolution; Binary star","score_opus":0.021013809620616563,"score_gpt":0.2404062822190432,"score_spread":0.21939247259842665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2604995907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98979867,0.0003346702,0.00542151,0.00011264337,0.0000041053518,0.000014620539,0.00020714969,0.000031865744,0.0040748203],"genre_scores_gemma":[0.99872833,0.00012729829,0.0006341661,0.000008060384,0.0000029149348,0.00000420313,0.000107008396,0.000009776672,0.00037839613],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986553,0.000026865342,0.000005709731,0.00004304068,0.00003297785,0.000025865065],"domain_scores_gemma":[0.9983607,0.0009613545,0.0002683247,0.00017254696,0.0001457546,0.00009128251],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061741157,0.00019726116,0.00023459301,0.0009075709,0.00047541884,0.000973675,0.0007659343,0.00046669054,0.002241876],"category_scores_gemma":[0.0034651866,0.00020755868,0.00033378275,0.00047409625,0.0008025595,0.00085268123,0.00058213214,0.0004647893,0.0004937066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022027286,0.000048894217,0.82077247,0.00009634901,0.00006240588,0.00024057466,0.0006368405,0.07812221,0.007668365,0.061905716,0.00066891394,0.029556977],"study_design_scores_gemma":[0.000045199035,0.00013426431,0.71409464,0.000058789465,0.00005969101,0.00061861053,0.0007039309,0.21404204,0.00824481,0.056757193,0.005194826,0.00004601715],"about_ca_topic_score_codex":0.0042056255,"about_ca_topic_score_gemma":0.0036509233,"teacher_disagreement_score":0.0042056255,"about_ca_system_score_codex":0.0010475542,"about_ca_system_score_gemma":0.00018735405,"threshold_uncertainty_score":0.008362293},"labels":[],"label_agreement":null},{"id":"W2605570044","doi":"10.3847/1538-4357/aa68dd","title":"The Chandra Dust-scattering Halo of Galactic Center Transient Swift J174540.7–290015","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Halo; Galactic Center; Swift; Galactic halo; Brightness; Surface brightness; Binary number; Compact star","score_opus":0.018093810993087413,"score_gpt":0.2481210701135778,"score_spread":0.2300272591204904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2605570044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990839,0.000053819324,0.0001507579,0.000013860238,0.000004727641,0.0000024381575,0.00011337426,0.000026045236,0.0005510804],"genre_scores_gemma":[0.99940836,0.00001632756,0.00022269813,0.000008695035,0.000006692604,0.0000014597421,0.00022634387,0.000007444908,0.00010202984],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999416,0.0000029229827,0.0000030047902,0.000014537542,0.000016975178,0.00002103095],"domain_scores_gemma":[0.99965215,0.000033366963,0.00011181709,0.000042202326,0.000041405645,0.000119177355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013861763,0.00015514102,0.00021297505,0.00087860436,0.00037260805,0.00046642704,0.00025082708,0.00013282683,0.0009574745],"category_scores_gemma":[0.00034257126,0.00012768708,0.00022631373,0.0004697071,0.00029789313,0.00018150928,0.00047356597,0.0001812205,0.0001486816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092373736,0.00018904307,0.6068132,0.00012759933,0.00020303228,0.0039993655,0.0008363342,0.0029604284,0.36056468,0.0009445729,0.0018604746,0.02057744],"study_design_scores_gemma":[0.000014393286,0.0000698799,0.9902023,0.000008502866,0.000023649363,0.0006711276,0.00017981736,0.0017157884,0.0058749667,0.00008594234,0.0011410848,0.000012556705],"about_ca_topic_score_codex":0.004981381,"about_ca_topic_score_gemma":0.0067821643,"teacher_disagreement_score":0.004981381,"about_ca_system_score_codex":0.0003813819,"about_ca_system_score_gemma":0.00021403976,"threshold_uncertainty_score":0.009904742},"labels":[],"label_agreement":null},{"id":"W2605644516","doi":"10.3847/1538-4357/aa7cfd","title":"A New Limit on CMB Circular Polarization from SPIDER","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Cosmic microwave background; Polarization (electrochemistry); Polarization in astronomy; Stokes parameters; Circular polarization; Linear polarization; Cosmic background radiation; Telescope","score_opus":0.011946136723659542,"score_gpt":0.2535828893394687,"score_spread":0.24163675261580916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2605644516","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47189185,0.013160208,0.1769377,0.0046837893,0.0013097465,0.0001441152,0.015309079,0.008202905,0.30836052],"genre_scores_gemma":[0.96308076,0.0012690176,0.020745944,0.0019557225,0.00058159616,0.00018544788,0.008755737,0.00069167506,0.0027340488],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9969982,0.00035216432,0.000109015135,0.0007947692,0.0013698157,0.00037620246],"domain_scores_gemma":[0.99450666,0.0023271532,0.0006645613,0.0011932878,0.0007278883,0.0005803586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002676266,0.001120126,0.0010060832,0.002037475,0.0010885664,0.002801136,0.00129383,0.0013755183,0.007805464],"category_scores_gemma":[0.0065448373,0.00079849025,0.0008394535,0.0011009665,0.0011017417,0.002631405,0.0035318078,0.0028854213,0.0029692391],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002263415,0.00033063343,0.21620686,0.0017774119,0.0005361231,0.0022872165,0.0017253137,0.017169567,0.16354671,0.3313963,0.086891055,0.17586939],"study_design_scores_gemma":[0.0002961745,0.0004936333,0.15582658,0.0012136068,0.00028003755,0.0032320223,0.00048660333,0.070112355,0.14983393,0.29121134,0.3264179,0.0005958851],"about_ca_topic_score_codex":0.001509292,"about_ca_topic_score_gemma":0.001422319,"teacher_disagreement_score":0.007805464,"about_ca_system_score_codex":0.001207356,"about_ca_system_score_gemma":0.00056638045,"threshold_uncertainty_score":0.0261119},"labels":[],"label_agreement":null},{"id":"W2605733806","doi":"10.3847/1538-4357/aa6d67","title":"Prospects for Cherenkov Telescope Array Observations of the Young Supernova Remnant RX J1713.7−3946","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Argonne National Laboratory; Deutsches Elektronen-Synchrotron; Istituto Nazionale di Fisica Nucleare; State Committee of Science; Bergens Forskningsstiftelse; Institute for Cosmic Ray Research, University of Tokyo; Centre National de la Recherche Scientifique; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Ministère de l'Education Nationale, de l'Enseignement Superieur et de la Recherche; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Hrvatska Zaklada za Znanost; Narodowym Centrum Nauki; Japan Society for the Promotion of Science; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministerio de Ciencia, Tecnología e Innovación Productiva; Istituto Nazionale di Astrofisica; Durham University; Consejo Nacional de Investigaciones Científicas y Técnicas; Comisión Nacional de Energía Atómica, Gobierno de Argentina; Iowa State University; Ministerstvo Školství, Mládeže a Tělovýchovy; Bundesministerium für Bildung und Forschung; Fundação de Amparo à Pesquisa do Estado de São Paulo; Ministero dell’Istruzione, dell’Università e della Ricerca; European Commission; Royal Swedish Academy of Sciences; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; Barnard College; University of Oxford; Javna Agencija za Raziskovalno Dejavnost RS; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Max-Planck-Gesellschaft; University of Leicester; Grantová Agentura České Republiky; Leverhulme Trust; Vetenskapsrådet; U.S. Department of Energy; Georgia Institute of Technology; Centro para el Desarrollo Tecnológico Industrial; National Science Foundation","keywords":"Physics; Cherenkov Telescope Array; Supernova remnant; Cosmic ray; Astrophysics; Gamma ray; Supernova; Cherenkov radiation; Telescope; Astronomy; Spectral line; Particle acceleration; Electron; Nuclear physics; Optics","score_opus":0.025173730536882086,"score_gpt":0.24944610685227028,"score_spread":0.2242723763153882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2605733806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942379,0.00006782757,0.0031169085,0.000237659,0.000015358128,0.000018851515,0.00027686305,0.00008546542,0.0019430249],"genre_scores_gemma":[0.9977514,0.000038515853,0.0014170771,0.00003730475,0.0000060096913,0.000021407697,0.0005123328,0.000022332439,0.00019349791],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997918,0.00007928895,0.0000073552415,0.000035814755,0.000037072637,0.000048609872],"domain_scores_gemma":[0.9989324,0.0004868344,0.00012760391,0.00011749304,0.00014555185,0.00019004913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017036727,0.0003838055,0.00058950874,0.0003346657,0.0006978971,0.00085620536,0.00086894,0.00065775955,0.0011458761],"category_scores_gemma":[0.0028427572,0.00037262667,0.00097051216,0.00045083096,0.0006321495,0.0005231961,0.0006136347,0.00068615837,0.00015706845],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023303457,0.0001248663,0.0642281,0.000017830927,0.00014238138,0.00016457347,0.00005679528,0.9272236,0.0024839095,0.003575012,0.00044513133,0.0013046948],"study_design_scores_gemma":[0.00015665835,0.00016475782,0.021842007,0.000009712757,0.000058512156,0.000039353883,0.000092736926,0.9735381,0.0013799253,0.0020886871,0.00060006167,0.000029549085],"about_ca_topic_score_codex":0.013888312,"about_ca_topic_score_gemma":0.008223756,"teacher_disagreement_score":0.013888312,"about_ca_system_score_codex":0.0011093841,"about_ca_system_score_gemma":0.0009819382,"threshold_uncertainty_score":0.027614892},"labels":[],"label_agreement":null},{"id":"W2605820156","doi":"10.3847/1538-4357/aa67db","title":"Action-based Dynamical Modeling for the Milky Way Disk: The Influence of Spiral Arms","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Spiral galaxy; Milky Way; Stars; Galaxy; Astrophysics; Gravitational potential; Gravitation; Astronomy","score_opus":0.023996046987053515,"score_gpt":0.2708844774127369,"score_spread":0.2468884304256834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2605820156","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9353103,0.00025618493,0.059274632,0.0003198492,0.000015262607,0.000033685326,0.00068064313,0.00037464497,0.0037347474],"genre_scores_gemma":[0.9941702,0.00007768135,0.004990058,0.00002705553,0.000008534357,0.000026094642,0.00027494715,0.000059636917,0.00036589516],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990857,0.00003475735,0.0000047161006,0.000022519007,0.000013909884,0.000015470978],"domain_scores_gemma":[0.99926895,0.0003942399,0.000102692444,0.00008623194,0.000081405706,0.00006651888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040844534,0.00043959753,0.00042930178,0.0006738847,0.0003624228,0.0008052668,0.0010259427,0.00077348144,0.0014382463],"category_scores_gemma":[0.0025980116,0.00030981377,0.00076122716,0.00037105614,0.00047515632,0.000658759,0.00055737514,0.00041585753,0.00024628686],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000014529236,0.0000065860554,0.0047013983,0.000009088063,0.000017751292,0.00003828389,0.000039434715,0.99171793,0.00036667357,0.0015900886,0.0001001108,0.0013979934],"study_design_scores_gemma":[0.0000028034665,0.000003939273,0.0005621468,0.0000020454263,0.0000018917356,0.000006713376,0.000006534419,0.9984914,0.00005252549,0.0007555261,0.00011187744,0.0000025737688],"about_ca_topic_score_codex":0.03207832,"about_ca_topic_score_gemma":0.010256755,"teacher_disagreement_score":0.03207832,"about_ca_system_score_codex":0.000796829,"about_ca_system_score_gemma":0.0005406141,"threshold_uncertainty_score":0.06378323},"labels":[],"label_agreement":null},{"id":"W2605880790","doi":"10.3847/1538-4357/aa6d0f","title":"Absolute Magnitudes of Seismic Red Clumps in the Kepler Field and SAGA: The Age Dependency of the Distance Scale","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Kepler; Scale (ratio); Astrophysics; Astronomy; Absolute magnitude; Absolute (philosophy); Absolute scale; Field (mathematics); Magnitude (astronomy); Red shift; Stars; Galaxy; Atomic physics","score_opus":0.012690001045896737,"score_gpt":0.23353598722208915,"score_spread":0.22084598617619242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2605880790","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99750644,0.00008307376,0.00065093546,0.00001749659,0.0000034359737,0.0000018878987,0.00039007457,0.00002946298,0.0013172576],"genre_scores_gemma":[0.9989926,0.000025093657,0.0002812795,0.000008835103,0.000003608412,0.0000017558548,0.00052932213,0.000008912391,0.0001486409],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972314,0.000041461142,0.000024543837,0.00009680382,0.00007279537,0.000041160856],"domain_scores_gemma":[0.997232,0.0007548157,0.0009478496,0.00035989407,0.00042147381,0.00028396843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059946725,0.00020687368,0.00020850163,0.002166737,0.00018525207,0.00069072214,0.00024385934,0.000274281,0.0010690637],"category_scores_gemma":[0.0028413786,0.00016220596,0.00013717258,0.00095320155,0.00034836057,0.00047994,0.00047942402,0.00022030639,0.0004662539],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007626604,0.000018768475,0.9832977,0.000020092302,0.0000255863,0.00003571665,0.00014328003,0.0009718209,0.0062623615,0.0004342979,0.00022615443,0.008488058],"study_design_scores_gemma":[0.00000214018,0.000015511914,0.9976949,0.000005460905,0.0000048069805,0.000029191773,0.000040599323,0.0011571817,0.00066680013,0.00013777052,0.00024243463,0.0000032951773],"about_ca_topic_score_codex":0.0020949575,"about_ca_topic_score_gemma":0.0024200778,"teacher_disagreement_score":0.002166737,"about_ca_system_score_codex":0.00026620337,"about_ca_system_score_gemma":0.00010503942,"threshold_uncertainty_score":0.00416559},"labels":[],"label_agreement":null},{"id":"W2606167848","doi":"10.3847/1538-4357/aa689f","title":"First Discoveries of z &gt; 6 Quasars with the DECam Legacy Survey and UKIRT Hemisphere Survey","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Vedecká Grantová Agentúra MŠVVaŠ SR a SAV; National Natural Science Foundation of China; Chinese Academy of Sciences; Smithsonian Institution; National Science Foundation","keywords":"Quasar; Sky; Redshift; Absolute magnitude; Magnitude (astronomy); Population; Luminosity","score_opus":0.011982321424172717,"score_gpt":0.22586694763207557,"score_spread":0.21388462620790286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606167848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98962337,0.00046232707,0.00059449207,0.0002195194,0.000018138575,0.000023324512,0.0028873214,0.00006123101,0.006110227],"genre_scores_gemma":[0.9953412,0.00019542099,0.0009935779,0.000086666696,0.000037210346,0.000011790801,0.002433658,0.000010813266,0.00088967825],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995395,0.000067582696,0.00003137006,0.00008810343,0.0001618109,0.00011172594],"domain_scores_gemma":[0.9981585,0.00018222637,0.0005866256,0.0002524882,0.0003945794,0.00042557047],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009517623,0.00017557306,0.00017768871,0.001670057,0.00033719846,0.0006436899,0.0003810944,0.00021249715,0.0011916221],"category_scores_gemma":[0.001686991,0.00015360588,0.00015435425,0.0011950936,0.00025297614,0.00045916295,0.0014343632,0.00025126536,0.00037766618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018438288,0.000019306444,0.96879935,0.000026257838,0.00003519274,0.00046179566,0.00075267436,0.000034733042,0.006937381,0.00022828583,0.0015604574,0.020960215],"study_design_scores_gemma":[0.0000032401408,0.000018022385,0.9963644,0.000004858905,0.0000068180557,0.00019262946,0.00008810636,0.000030283705,0.000320981,0.000023663557,0.0029446252,0.0000024688604],"about_ca_topic_score_codex":0.008213258,"about_ca_topic_score_gemma":0.022926647,"teacher_disagreement_score":0.008213258,"about_ca_system_score_codex":0.0004103569,"about_ca_system_score_gemma":0.00015100463,"threshold_uncertainty_score":0.016330898},"labels":[],"label_agreement":null},{"id":"W2606415625","doi":"10.3847/1538-4357/aa6842","title":"X-Ray Insights into the Nature of Quasars with Redshifted Broad Absorption Lines","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Astrophysics; Physics; Redshift; Spectral line; Absorption (acoustics); Emission spectrum; Absorption spectroscopy; Accretion (finance); Astronomy; Galaxy; Optics","score_opus":0.006355483166889378,"score_gpt":0.22546258235025377,"score_spread":0.21910709918336438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606415625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988558,0.00006468123,0.00033370176,0.000012842591,9.844929e-7,0.0000013859024,0.00004673695,0.0000147503,0.0006690557],"genre_scores_gemma":[0.9998292,0.000009388829,0.000085434884,0.0000047866088,0.0000012770153,4.0655453e-7,0.000025659127,0.0000010422943,0.000042839198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999317,0.000008695028,0.0000043851833,0.000012347194,0.000016637543,0.00002618112],"domain_scores_gemma":[0.99925214,0.00012833854,0.00032789717,0.00006705514,0.00007608574,0.00014842494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002777668,0.00016289958,0.00012952481,0.00091043377,0.00025145157,0.00055896613,0.00021690423,0.00016526089,0.001063293],"category_scores_gemma":[0.0004817172,0.000111553476,0.00012659149,0.00034744365,0.00034124477,0.00035024455,0.00043289943,0.00020614869,0.00015506618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011432501,0.000042495714,0.9398481,0.0000237643,0.00003180567,0.00021510852,0.0003049257,0.0004692885,0.052901883,0.00086828065,0.00010248643,0.005077377],"study_design_scores_gemma":[0.000003406225,0.000069548674,0.9943862,0.0000044611425,0.000015845926,0.00036175063,0.00025883262,0.0010947092,0.00311718,0.00033648405,0.00034624664,0.0000052188725],"about_ca_topic_score_codex":0.00080736895,"about_ca_topic_score_gemma":0.0013004731,"teacher_disagreement_score":0.001063293,"about_ca_system_score_codex":0.0001304945,"about_ca_system_score_gemma":0.00007160198,"threshold_uncertainty_score":0.0035570264},"labels":[],"label_agreement":null},{"id":"W2606504280","doi":"10.3847/1538-4357/aa6983","title":"Morphological Properties of the Crab Nebula: A Detailed Multiwavelength Study Based on New VLA, HST, Chandra, and XMM-Newton Images","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Nebula; Crab Nebula; Angular resolution (graph drawing); Pulsar; Astronomy; Radio spectrum; Stars","score_opus":0.028336600052944236,"score_gpt":0.30772417085396664,"score_spread":0.2793875708010224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606504280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967933,0.00057798444,0.00083311595,0.0000151274735,0.0000037508134,0.000016961934,0.00061695575,0.00005910565,0.0010836218],"genre_scores_gemma":[0.9959663,0.00023421137,0.0022423808,0.000019495003,0.000014922782,0.000013481249,0.0011573116,0.000042744803,0.00030915282],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998796,0.00000868169,0.000010095842,0.000041361658,0.000037407757,0.000022841881],"domain_scores_gemma":[0.99958295,0.000041599404,0.00014784532,0.00007743825,0.00006548707,0.00008459418],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002558905,0.00020673191,0.00031993724,0.002636394,0.00031259612,0.00067440706,0.00023965418,0.00017724452,0.0007020965],"category_scores_gemma":[0.00034799246,0.00025249974,0.00042392453,0.0010485207,0.00022110606,0.00032386754,0.00047201387,0.00017667301,0.00032547212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018534817,0.00010653653,0.7392518,0.00010443947,0.00018851366,0.0011151775,0.00044479553,0.0014714384,0.23512547,0.00016566704,0.00036176882,0.021479078],"study_design_scores_gemma":[0.0000019758807,0.00001781202,0.99721587,0.0000030100985,0.000012514586,0.00034300904,0.000034516,0.00042704315,0.0015583383,0.000014706883,0.00036662482,0.0000046141968],"about_ca_topic_score_codex":0.0011676046,"about_ca_topic_score_gemma":0.0018793428,"teacher_disagreement_score":0.002636394,"about_ca_system_score_codex":0.00017905819,"about_ca_system_score_gemma":0.000092605515,"threshold_uncertainty_score":0.002348721},"labels":[],"label_agreement":null},{"id":"W2606762111","doi":"10.3847/1538-4357/aa6bfa","title":"Thermal Feedback in the High-mass Star- and Cluster-forming Region W51","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Deutsche Forschungsgemeinschaft; Associated Universities; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Star (game theory); Astrophysics; Astronomy; Cluster (spacecraft); Thermal; Star cluster; High mass; Thermal emission; Stars; Meteorology","score_opus":0.014625684013403766,"score_gpt":0.2432404869083425,"score_spread":0.2286148028949387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2606762111","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996099,0.000020113688,0.00004312202,0.000007008583,3.823038e-7,9.213359e-7,0.000018285518,0.0000039940974,0.00029639946],"genre_scores_gemma":[0.99984884,0.0000063701177,0.00003405735,0.0000037169366,5.839757e-7,6.862428e-7,0.000026882166,8.72883e-7,0.00007800148],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.000005805196,0.000003848566,0.00002218705,0.000009969958,0.000021255555],"domain_scores_gemma":[0.9998202,0.000025845102,0.00007325646,0.00001537058,0.000017216287,0.000048165017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000083634615,0.00013804581,0.00017020218,0.00024854505,0.00033213434,0.00041918212,0.00024772814,0.00023682485,0.0012003473],"category_scores_gemma":[0.00037242568,0.00013914004,0.00009846886,0.00017931806,0.00027726966,0.00019258414,0.00042478743,0.00010867087,0.00024073973],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024250924,0.000066178945,0.8588141,0.000035292003,0.000041847663,0.00048064522,0.00055876153,0.0013302566,0.12918702,0.00045450559,0.00028448403,0.0085043395],"study_design_scores_gemma":[0.0000053576737,0.000037327034,0.99687445,0.000003665437,0.0000067559104,0.00012795346,0.00012291335,0.0012410324,0.0012936023,0.00008904668,0.00019538074,0.000002549361],"about_ca_topic_score_codex":0.0062518204,"about_ca_topic_score_gemma":0.009366844,"teacher_disagreement_score":0.0062518204,"about_ca_system_score_codex":0.00035251706,"about_ca_system_score_gemma":0.00011736683,"threshold_uncertainty_score":0.012430847},"labels":[],"label_agreement":null},{"id":"W2607061531","doi":"10.3847/1538-4357/aa8b1c","title":"GCM Simulations of Unstable Climates in the Habitable Zone","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Planetary Science and Exploration","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"GCM transcription factors; Circumstellar habitable zone; Climatology; Planetary habitability; Planet; Climate state; Climate model; Climate change; Environmental science; General Circulation Model; Geology; Atmospheric sciences; Astrobiology; Terrestrial planet; Physics; Exoplanet; Global warming; Astrophysics; Effects of global warming","score_opus":0.020678765153453346,"score_gpt":0.2594143307435204,"score_spread":0.23873556559006703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2607061531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99671435,0.000046352747,0.0010890668,0.00014641293,0.000016993392,0.000009471867,0.0002525982,0.00006641346,0.0016583634],"genre_scores_gemma":[0.9986547,0.00002222463,0.0008925089,0.000031398777,0.000004785539,0.000011637208,0.00016603949,0.000016029066,0.00020056264],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999913,0.000027080458,0.000004391526,0.00001509038,0.000013494794,0.00002694868],"domain_scores_gemma":[0.99947435,0.00025112834,0.000053138905,0.0000570676,0.00005454571,0.00010974794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003258183,0.00032038684,0.0005207614,0.00043076032,0.00052218576,0.0008757201,0.0008390365,0.0012187336,0.0019009472],"category_scores_gemma":[0.0018268828,0.00022822231,0.00046073392,0.0006364711,0.0008992253,0.0004612876,0.00076026114,0.00077589735,0.00010528471],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011959555,0.00009139083,0.011867098,0.00002484944,0.00005979632,0.00012483522,0.000091930706,0.9831549,0.0013788949,0.0016664999,0.00030619177,0.0011140394],"study_design_scores_gemma":[0.00005292838,0.000033357832,0.0036495256,0.000005179544,0.000010527385,0.000008384371,0.000053906813,0.9952023,0.00024037025,0.00049672014,0.00023724562,0.000009477841],"about_ca_topic_score_codex":0.033169813,"about_ca_topic_score_gemma":0.016783373,"teacher_disagreement_score":0.033169813,"about_ca_system_score_codex":0.000903405,"about_ca_system_score_gemma":0.00070227217,"threshold_uncertainty_score":0.06595349},"labels":[],"label_agreement":null},{"id":"W2607177416","doi":"10.3847/1538-4357/aa6a1e","title":"The Correlation between Mixing Length and Metallicity on the Giant Branch: Implications for Ages in the Gaia Era","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Economía y Competitividad; Centre National d’Etudes Spatiales; Generalitat de Catalunya; University of Oxford; York University; Universidad Nacional Autónoma de México; Magyar Tudományos Akadémia; Space Telescope Science Institute; Villum Fonden; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Stellar Astrophysics Centre; Danmarks Grundforskningsfond; Leibniz-Gemeinschaft; University of Notre Dame; Ohio State University; National Research Foundation; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; National Science Foundation; Smithsonian Institution; U.S. Department of Energy; New Mexico State University; University of Portsmouth; Vanderbilt University; National Research, Development and Innovation Office; Science Mission Directorate; Yale University","keywords":"Metallicity; Physics; Astrophysics; Mixing (physics); Convective mixing; Red-giant branch; Stars; Red giant; Stellar mass; Convection; Astronomy; Star formation; Meteorology","score_opus":0.033750616214678064,"score_gpt":0.2767050019463723,"score_spread":0.24295438573169426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2607177416","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99546105,0.00060722145,0.00069153594,0.0005045142,0.000017993374,0.0000014723887,0.00037167798,0.00003289708,0.0023114884],"genre_scores_gemma":[0.9993685,0.000079257494,0.00015190896,0.000028369977,0.000012561374,5.990782e-7,0.000121796926,0.000010395289,0.00022670122],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986255,0.00002852397,0.0000108000995,0.000047412836,0.00002345132,0.000027129237],"domain_scores_gemma":[0.9977196,0.00088806305,0.0006511975,0.0002783402,0.00020668731,0.00025611912],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008394707,0.00016325785,0.00017155585,0.0008171382,0.00030144406,0.0010380034,0.00030873663,0.00030068288,0.0023335835],"category_scores_gemma":[0.0048352485,0.000099181096,0.00018143817,0.00066725595,0.0004966983,0.0007587785,0.00052206457,0.0004900318,0.00043055462],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016216366,0.0000074675777,0.9871999,0.00001532344,0.000047626178,0.00007663299,0.00018029485,0.0008851332,0.0029182653,0.0015468653,0.00024689257,0.00671339],"study_design_scores_gemma":[0.000004443456,0.000022766108,0.99434316,0.000010139541,0.000029058876,0.000083872656,0.00013150786,0.0017792276,0.0009495845,0.0015185341,0.0011221465,0.0000055814166],"about_ca_topic_score_codex":0.002451788,"about_ca_topic_score_gemma":0.0025420757,"teacher_disagreement_score":0.002451788,"about_ca_system_score_codex":0.0003886629,"about_ca_system_score_gemma":0.000138969,"threshold_uncertainty_score":0.007806599},"labels":[],"label_agreement":null},{"id":"W2607255761","doi":"10.3847/1538-4357/aa901a","title":"A Rogues’ Gallery of Andromeda's Dwarf Galaxies. I. A Predominance of Red Horizontal Branches","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Andromeda; Astrophysics; Dwarf spheroidal galaxy; Astronomy; Dwarf galaxy; Galaxy; Milky Way; Globular cluster; Local Group; Elliptical galaxy; Accretion (finance); Star formation; Interacting galaxy","score_opus":0.009179142060882517,"score_gpt":0.21970563809813878,"score_spread":0.21052649603725626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2607255761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903716,0.00062065053,0.00035618347,0.00011991405,0.000007549945,0.000006375475,0.00026566876,0.00004492508,0.008207152],"genre_scores_gemma":[0.99801135,0.000089340414,0.00020097166,0.000047503345,0.000011027036,0.0000023360078,0.00016533038,0.000008304644,0.0014637337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998387,0.000024771185,0.000009561078,0.000050271825,0.00003195286,0.000044733457],"domain_scores_gemma":[0.9993648,0.00010076658,0.00020402594,0.00019071689,0.000041541647,0.00009813763],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000339421,0.00015830001,0.00018038042,0.0017655191,0.000676485,0.00064918416,0.00019138039,0.00015971565,0.004156238],"category_scores_gemma":[0.00056555757,0.000100123274,0.00016756756,0.00059267605,0.0008757672,0.00039535994,0.0007603401,0.00014305348,0.00065147463],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028564018,0.00002342085,0.88946295,0.000069588525,0.00006171326,0.0010105517,0.004927615,0.00014027432,0.037852746,0.0063157105,0.0029283422,0.05692141],"study_design_scores_gemma":[0.0000028276418,0.000032185948,0.9865306,0.0000128010015,0.0000052385863,0.001725567,0.0006278186,0.00009121374,0.0010969286,0.000626668,0.009240219,0.000007952478],"about_ca_topic_score_codex":0.00187795,"about_ca_topic_score_gemma":0.00396854,"teacher_disagreement_score":0.004156238,"about_ca_system_score_codex":0.00015986223,"about_ca_system_score_gemma":0.000067918794,"threshold_uncertainty_score":0.0139039755},"labels":[],"label_agreement":null},{"id":"W2607720759","doi":"10.3847/1538-4357/aa7edf","title":"Limb Darkening and Planetary Transits: Testing Center-to-limb Intensity Variations and Limb-darkening Directly from Model Stellar Atmospheres","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Limb darkening; Exoplanet; Transit (satellite); Planet; Stellar atmosphere; Atmosphere (unit); Oscillation (cell signaling); Measure (data warehouse); Planetary system","score_opus":0.021744898129900173,"score_gpt":0.22839551108143422,"score_spread":0.20665061295153403,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2607720759","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961217,0.0000075788403,0.002877774,0.000008041149,0.0000023392865,0.0000073590845,0.00046121443,0.0001500358,0.0003638296],"genre_scores_gemma":[0.9977422,0.0000038763246,0.001592692,0.0000037702787,0.0000010543553,0.0000048126717,0.0005780284,0.000030421343,0.000043069947],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99977976,0.00007810819,0.000013539142,0.00006573136,0.000039036575,0.000023739622],"domain_scores_gemma":[0.99874556,0.0006600001,0.00014703009,0.00023073929,0.00013110293,0.00008553115],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006547774,0.0003230599,0.0001438283,0.00040385575,0.00021965557,0.00040130824,0.00037534145,0.00026665552,0.0007856008],"category_scores_gemma":[0.002231356,0.00012390783,0.00045119578,0.0004220862,0.00028959208,0.00031813417,0.00030335347,0.00024224947,0.00015934494],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008581104,0.0005032392,0.43828183,0.00007071304,0.00016732675,0.00010970501,0.00016521088,0.5018066,0.042864688,0.0011689392,0.00055798405,0.013445644],"study_design_scores_gemma":[0.00006165903,0.00041126588,0.23498684,0.000004958353,0.000035138655,0.00007763792,0.00007950824,0.7403786,0.023122126,0.00039417975,0.0004249846,0.00002317629],"about_ca_topic_score_codex":0.016297188,"about_ca_topic_score_gemma":0.011367424,"teacher_disagreement_score":0.016297188,"about_ca_system_score_codex":0.00054328114,"about_ca_system_score_gemma":0.0003530562,"threshold_uncertainty_score":0.03240466},"labels":[],"label_agreement":null},{"id":"W2608135358","doi":"10.3847/1538-4357/aa6f5f","title":"Evidence for Different Disk Mass Distributions between Early- and Late-type Be Stars in the BeSOS Survey","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Stars; Thick disk; Angular momentum; Thin disk; Stellar classification; Circumstellar disk; Be star; Stellar mass; Astronomy; Star formation; Galaxy","score_opus":0.08257197623781183,"score_gpt":0.3113116326471122,"score_spread":0.22873965640930038,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2608135358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99946064,0.000023356293,0.000095839736,0.000006133786,6.309634e-7,9.926902e-7,0.00012885938,0.0000035077987,0.00028007958],"genre_scores_gemma":[0.9994289,0.000021653961,0.000064559485,0.00000476339,0.0000013859625,0.0000012827448,0.00035898597,0.0000031276156,0.000115212715],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998055,0.000036816156,0.000022397224,0.00006152119,0.000040772527,0.000032989486],"domain_scores_gemma":[0.9991659,0.00013393082,0.00030984296,0.000074516494,0.000121416,0.00019449722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033686272,0.00019334548,0.00026797445,0.0011574962,0.00030244555,0.00057421345,0.00013883298,0.00016573715,0.0013133211],"category_scores_gemma":[0.0008852543,0.00015405988,0.00016799278,0.00056665315,0.00027635807,0.00029477582,0.00046030653,0.000113685855,0.0004299851],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001173508,0.000013650468,0.99504155,0.0000063719062,0.000014204749,0.00002982563,0.000114963106,0.00008321806,0.0033633867,0.000055950528,0.000044527067,0.001115094],"study_design_scores_gemma":[0.0000035626408,0.000023646578,0.9990013,0.0000023024852,0.0000049019027,0.00007614451,0.00019264076,0.00019780299,0.00028873165,0.000041985597,0.00016572609,0.0000011340597],"about_ca_topic_score_codex":0.0016276729,"about_ca_topic_score_gemma":0.0033402788,"teacher_disagreement_score":0.0016276729,"about_ca_system_score_codex":0.000121953206,"about_ca_system_score_gemma":0.00007992001,"threshold_uncertainty_score":0.004393518},"labels":[],"label_agreement":null},{"id":"W2608244452","doi":"10.3847/1538-4357/aaa3ef","title":"A Comparison of Maps and Power Spectra Determined from South Pole Telescope and Planck Data","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Multipole expansion; Sky; Telescope; Planck; Spectral density; Tilt (camera); Calibration; Angular resolution (graph drawing); Spectral line","score_opus":0.01725566679516569,"score_gpt":0.2531624790319939,"score_spread":0.23590681223682822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2608244452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99508506,0.00007201255,0.002619389,0.000038330294,0.000009172901,0.000007333822,0.0007745351,0.00014029253,0.0012538355],"genre_scores_gemma":[0.99623257,0.000034770146,0.0014689035,0.000011830184,0.0000120400455,0.000009007228,0.0020235241,0.000088241264,0.00011929391],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987754,0.00022561,0.00007145839,0.00040849968,0.00042618168,0.00009283613],"domain_scores_gemma":[0.9934535,0.0029663027,0.0010530535,0.0014231438,0.00092419656,0.00017974812],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019807382,0.00036960724,0.00031506064,0.002619432,0.00026255305,0.0011658347,0.0005584498,0.00042406277,0.0018434725],"category_scores_gemma":[0.012906985,0.00040491397,0.0006875008,0.0024353212,0.0005001654,0.0009922737,0.0011286573,0.00030768028,0.00045595827],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004729379,0.000036950198,0.94201905,0.000106448686,0.00094420713,0.00039219356,0.0004910503,0.015205148,0.016486162,0.0011249706,0.0009015666,0.02181928],"study_design_scores_gemma":[0.0000082344595,0.0000249887,0.986394,0.0000072220946,0.00006980831,0.00011979497,0.00008607034,0.009507476,0.00292224,0.0002686774,0.00057446776,0.00001715093],"about_ca_topic_score_codex":0.0027612676,"about_ca_topic_score_gemma":0.0018426075,"teacher_disagreement_score":0.0027612676,"about_ca_system_score_codex":0.00039118127,"about_ca_system_score_gemma":0.00015050253,"threshold_uncertainty_score":0.010475278},"labels":[],"label_agreement":null},{"id":"W2608320463","doi":"10.3847/1538-4357/aa832b","title":"Space Telescope and Optical Reverberation Mapping Project. VII. Understanding the Ultraviolet Anomaly in NGC 5548 with X-Ray Spectroscopy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; University of Leicester; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution; Consejo Nacional de Ciencia y Tecnología; National Science Foundation","keywords":"Physics; Astrophysics; Spectral line; Anomaly (physics); Emission spectrum; Spectroscopy; Ultraviolet; Line (geometry); South Atlantic Anomaly; Astronomy; Magnetosphere; Plasma; Optics","score_opus":0.02716529802469103,"score_gpt":0.2565743063233268,"score_spread":0.22940900829863575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2608320463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99544466,0.000099748,0.0015209318,0.00011598159,0.000009121092,0.000010264688,0.0012784383,0.0001374843,0.001383365],"genre_scores_gemma":[0.9950236,0.00004242377,0.0029278279,0.000023776573,0.000010834049,0.000005947466,0.00141186,0.00002681284,0.0005270618],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989986,0.000015011553,0.000006637581,0.000021758602,0.000027714676,0.000028904966],"domain_scores_gemma":[0.99962115,0.000033957625,0.00014443825,0.00008309656,0.00005401568,0.00006330913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002817054,0.00025752324,0.00013990664,0.00072927814,0.00018834398,0.00037137498,0.00025459976,0.00017952884,0.0012729554],"category_scores_gemma":[0.000570593,0.00012204197,0.00017544889,0.0004919952,0.00013682117,0.00041699168,0.0004003076,0.00021979866,0.00029174561],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026447832,0.00011685295,0.87429404,0.00005030885,0.00007004356,0.00047220406,0.00027746023,0.0017272424,0.082148165,0.00043876603,0.002315588,0.03782499],"study_design_scores_gemma":[0.00001140573,0.00006369121,0.98349124,0.0000064783385,0.000024619962,0.00025772638,0.00007330079,0.004532443,0.008906034,0.0002771548,0.0023501453,0.000005754172],"about_ca_topic_score_codex":0.0036816488,"about_ca_topic_score_gemma":0.008477597,"teacher_disagreement_score":0.0036816488,"about_ca_system_score_codex":0.00016714596,"about_ca_system_score_gemma":0.000119431046,"threshold_uncertainty_score":0.0073204637},"labels":[],"label_agreement":null},{"id":"W2609097503","doi":"10.3847/1538-4357/aa6c67","title":"Cloud Structure of Three Galactic Infrared Dark Star-forming Regions from Combining Ground- and Space-based Bolometric Observations","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Star formation; Molecular cloud; Luminosity; Stars; Galaxy","score_opus":0.03025300392708608,"score_gpt":0.25022039726443424,"score_spread":0.21996739333734816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2609097503","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985733,0.000026650805,0.0010748672,0.0000033923534,6.949822e-7,0.0000050900735,0.00014427128,0.00002575705,0.00014594715],"genre_scores_gemma":[0.9977685,0.000012956777,0.0016555701,0.0000034742304,0.0000017708522,0.0000031049858,0.0005153801,0.0000067398673,0.000032425243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999858,0.000016255184,0.0000081647695,0.000046824105,0.00003794124,0.00003281055],"domain_scores_gemma":[0.99968815,0.00005009117,0.00007585653,0.00005465481,0.00005796912,0.000073336116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043292335,0.00024358073,0.0002988965,0.0013606838,0.0002356262,0.0006748945,0.00045636896,0.00024093258,0.0003332648],"category_scores_gemma":[0.0005036679,0.00023980206,0.0005651512,0.0011089229,0.00016391797,0.00025924697,0.00044942682,0.00014590222,0.00009235629],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016792616,0.00008000074,0.9100928,0.000031417963,0.00026845097,0.00023728542,0.00019875368,0.02178703,0.050267782,0.00026148412,0.00016291195,0.01644412],"study_design_scores_gemma":[0.000015204256,0.000032513162,0.9288297,0.0000065755644,0.000116671334,0.0000777312,0.00011028914,0.064491645,0.0059232228,0.00014895105,0.0002340948,0.000013366008],"about_ca_topic_score_codex":0.013619247,"about_ca_topic_score_gemma":0.018857446,"teacher_disagreement_score":0.013619247,"about_ca_system_score_codex":0.0005951469,"about_ca_system_score_gemma":0.00028518468,"threshold_uncertainty_score":0.02707994},"labels":[],"label_agreement":null},{"id":"W2609502880","doi":"10.3847/1538-4357/aa6d58","title":"The Green Bank Ammonia Survey: First Results of NH<sub>3</sub> Mapping of the Gould Belt","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Victoria; University of Alberta; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Green Bank Telescope; Emission spectrum; Ammonia; Southern Hemisphere; Kinetic energy; Galaxy; Northern Hemisphere; Line-of-sight","score_opus":0.020824472590327926,"score_gpt":0.24084171243808228,"score_spread":0.22001723984775434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2609502880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9603156,0.00094561063,0.00095292303,0.0002989818,0.00001658557,0.00007113091,0.02779754,0.00026233454,0.009339275],"genre_scores_gemma":[0.94642675,0.00095206784,0.0077189268,0.00046881076,0.000053833523,0.000122035046,0.039540093,0.00016716203,0.0045503858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966836,0.00005779806,0.0000147198725,0.000066615255,0.00011446058,0.00007802177],"domain_scores_gemma":[0.9991165,0.000098724835,0.0001750042,0.00012517847,0.00025761686,0.00022700486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005172204,0.0002830491,0.00022818141,0.0016206052,0.00035345327,0.0004844562,0.00039134987,0.00023424231,0.0017091295],"category_scores_gemma":[0.0006532372,0.00015091855,0.00021375768,0.0013653499,0.00021270048,0.00028423461,0.0008587955,0.00022563373,0.000760944],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028833217,0.000066257664,0.9336001,0.00010564001,0.00010695306,0.00030572643,0.0005418394,0.00074024376,0.011298667,0.00020584506,0.01172257,0.041017745],"study_design_scores_gemma":[0.000009718881,0.000018841854,0.99034715,0.00002359067,0.000012555403,0.000044070563,0.00015149382,0.0002956658,0.00076106965,0.000045947487,0.008281567,0.000008333988],"about_ca_topic_score_codex":0.120281376,"about_ca_topic_score_gemma":0.26237166,"teacher_disagreement_score":0.120281376,"about_ca_system_score_codex":0.0010921047,"about_ca_system_score_gemma":0.00066505076,"threshold_uncertainty_score":0.2391625},"labels":[],"label_agreement":null},{"id":"W2609640656","doi":"10.3847/1538-4357/aa689b","title":"Luminous Infrared Galaxies with the Submillimeter Array. V. Molecular Gas in Intermediate to Late-stage Mergers","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Luminous infrared galaxy; Milky Way; Infrared; Interstellar medium; Submillimeter Array; Line (geometry); Far infrared","score_opus":0.006741650544414474,"score_gpt":0.21239690473645786,"score_spread":0.2056552541920434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2609640656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9893706,0.0008753103,0.0009092945,0.00009660277,0.000012527435,0.0000135753635,0.0014538387,0.00014999218,0.0071184416],"genre_scores_gemma":[0.99752694,0.00009134138,0.00091256056,0.000041835126,0.00002118181,0.000008313558,0.00067055365,0.0000074441996,0.0007199659],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999869,0.000015504498,0.0000058537667,0.000049436756,0.000028082704,0.000032140128],"domain_scores_gemma":[0.999602,0.000039073657,0.00020088101,0.000034139983,0.000025219813,0.00009865015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023502129,0.0002178828,0.00015939055,0.0011606142,0.00025593006,0.0007090434,0.000222764,0.00020101682,0.0023748134],"category_scores_gemma":[0.0003808282,0.00010715995,0.00019236372,0.00081088365,0.00016921558,0.00037324245,0.00035176828,0.00029599125,0.00045394388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101684214,0.000037567912,0.9660987,0.000021445516,0.000036994006,0.000118524076,0.00017620064,0.00024462782,0.017174372,0.0003915863,0.000963405,0.014634822],"study_design_scores_gemma":[0.0000018267297,0.000009546583,0.9982895,0.0000030376336,0.0000056038675,0.000058576024,0.00003530968,0.00013831643,0.00055402453,0.000035863333,0.0008659663,0.000002317279],"about_ca_topic_score_codex":0.0050507286,"about_ca_topic_score_gemma":0.009897769,"teacher_disagreement_score":0.0050507286,"about_ca_system_score_codex":0.0002611144,"about_ca_system_score_gemma":0.00007886826,"threshold_uncertainty_score":0.010042667},"labels":[],"label_agreement":null},{"id":"W2609771036","doi":"10.3847/1538-4357/aa88c0","title":"The EDGE–CALIFA Survey: Variations in the Molecular Gas Depletion Time in Local Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galaxy; Stars; Gravitational potential; Drop (telecommunication); Luminous infrared galaxy; Star formation; Enhanced Data Rates for GSM Evolution; Gravitation","score_opus":0.008384952023582574,"score_gpt":0.2249329172941747,"score_spread":0.2165479652705921,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2609771036","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979699,0.00004937722,0.000034535216,0.000012965376,7.6578385e-7,0.0000025609202,0.0012768232,0.0000091134825,0.00064401457],"genre_scores_gemma":[0.99753016,0.000035790286,0.00011597756,0.000012297703,0.0000031570944,0.0000051991315,0.0019418909,0.0000047805784,0.0003507507],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998155,0.000020057538,0.000008011152,0.0000800313,0.000037411643,0.000038994025],"domain_scores_gemma":[0.9983394,0.00018256523,0.0004520287,0.00018022502,0.00043961353,0.00040612245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029796813,0.00014839125,0.00024779097,0.0015596783,0.0003311719,0.0005887098,0.00032322164,0.00020421055,0.0012812194],"category_scores_gemma":[0.0008002513,0.00016265994,0.00014831529,0.0012071846,0.0002549578,0.00024872072,0.0005726953,0.00016855983,0.00027158667],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000778982,0.000012287939,0.9960588,0.000007627508,0.00002212709,0.00002900283,0.00013303605,0.00006838483,0.001763134,0.000020377685,0.00021636263,0.0015910795],"study_design_scores_gemma":[0.0000011437185,0.000004321761,0.99974555,0.000001041445,0.0000025857755,0.000011115096,0.000040711144,0.000042858825,0.000057052064,0.0000015855595,0.00009118372,8.1576366e-7],"about_ca_topic_score_codex":0.061423354,"about_ca_topic_score_gemma":0.115720645,"teacher_disagreement_score":0.061423354,"about_ca_system_score_codex":0.0006935225,"about_ca_system_score_gemma":0.000272757,"threshold_uncertainty_score":0.122131646},"labels":[],"label_agreement":null},{"id":"W2609986691","doi":"10.3847/1538-4357/aa6a55","title":"Numerical Test of Analytical Theories for Perpendicular Diffusion in Small Kubo Number Turbulence","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Turbulence; Mean free path; Statistical physics; Nonlinear system; Kubo formula; Magnetohydrodynamic turbulence; K-epsilon turbulence model; K-omega turbulence model; Test particle; Classical mechanics; Diffusion; Gyrokinetics; Magnetohydrodynamics; Mechanics; Magnetic field; Quantum mechanics; Scattering; Plasma","score_opus":0.008897105218873746,"score_gpt":0.2574114469525571,"score_spread":0.24851434173368334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2609986691","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9766436,0.0002376438,0.014888186,0.00034684702,0.000052002477,0.000049263792,0.0001329368,0.00014911688,0.0075002746],"genre_scores_gemma":[0.9950553,0.000046305788,0.0043551284,0.000017082502,0.000007963952,0.00002533332,0.000054282384,0.000016303145,0.0004222375],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997452,0.00009241581,0.000015425536,0.000024013701,0.000072204704,0.00005071953],"domain_scores_gemma":[0.9977307,0.0013855043,0.00028010344,0.00018898853,0.00027372706,0.00014106598],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008264459,0.00053332315,0.0006055996,0.0007357281,0.0006052315,0.0007522133,0.0009972858,0.00079932535,0.0012210336],"category_scores_gemma":[0.00413735,0.00022710094,0.00053051003,0.00054618175,0.0011124935,0.0006742178,0.00069976284,0.0006925259,0.00008767389],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018713475,0.00020184983,0.0061742137,0.00009353977,0.000050811843,0.00021601222,0.00011496363,0.96527374,0.003993708,0.021199849,0.00047243794,0.0020217474],"study_design_scores_gemma":[0.000011804877,0.000025796224,0.00027279876,0.000002538468,0.0000026529242,0.000005529253,0.000009099625,0.99858534,0.0003628508,0.0006847168,0.000033094468,0.0000037688615],"about_ca_topic_score_codex":0.009240557,"about_ca_topic_score_gemma":0.0030019372,"teacher_disagreement_score":0.009240557,"about_ca_system_score_codex":0.0008216685,"about_ca_system_score_gemma":0.0006357006,"threshold_uncertainty_score":0.018373549},"labels":[],"label_agreement":null},{"id":"W2610068359","doi":"10.3847/1538-4357/aa6f11","title":"Weather on Other Worlds. IV. Hα Emission and Photometric Variability Are Not Correlated in L0–T8 Dwarfs","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Stellar classification; Brown dwarf; Photometry (optics); Photometric system; Flux (metallurgy); Spectral line; Starspot; Light curve","score_opus":0.01501990088663037,"score_gpt":0.2472916243827251,"score_spread":0.2322717234960947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2610068359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9009087,0.0014290268,0.0006656184,0.0017797861,0.00034454197,0.000025457815,0.0020255633,0.00011607455,0.09270526],"genre_scores_gemma":[0.9685079,0.0006773817,0.00035603577,0.0005861121,0.00014606425,0.0000069504354,0.00095285923,0.000033902368,0.028732877],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987805,0.000014628027,0.00001044528,0.000030758176,0.000024346484,0.00004174627],"domain_scores_gemma":[0.999443,0.000039139413,0.00017671801,0.000079355224,0.000078209916,0.00018362871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016695178,0.00008996671,0.00014212957,0.00035350077,0.0007363349,0.0009517161,0.00012963182,0.00017471284,0.016629368],"category_scores_gemma":[0.00062386796,0.000051958457,0.00010082278,0.00055488147,0.0003798532,0.00060025824,0.00059355225,0.00030587718,0.0034938331],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045294416,0.00012482949,0.7884236,0.00018926953,0.00013286356,0.0018526583,0.004978515,0.00045479892,0.016281176,0.007210538,0.029675387,0.15022337],"study_design_scores_gemma":[0.000013793794,0.00009385721,0.8191996,0.000071527385,0.00002099667,0.0012099729,0.004775547,0.00018545362,0.0014142698,0.0017276958,0.17126907,0.000018227007],"about_ca_topic_score_codex":0.0055433917,"about_ca_topic_score_gemma":0.010089615,"teacher_disagreement_score":0.016629368,"about_ca_system_score_codex":0.00028155264,"about_ca_system_score_gemma":0.0001929212,"threshold_uncertainty_score":0.055630803},"labels":[],"label_agreement":null},{"id":"W2610128407","doi":"10.3847/1538-4357/aa9af3","title":"The Onset of Thermally Unstable Cooling from the Hot Atmospheres of Giant Galaxies in Clusters: Constraints on Feedback Models","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":97,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Thermal; Galaxy cluster; Isentropic process; Gravitation; Cluster (spacecraft); Entropy (arrow of time); Acceleration","score_opus":0.014520320465187808,"score_gpt":0.22479129066905526,"score_spread":0.21027097020386745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2610128407","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99853945,0.000041370207,0.0007195035,0.000035494406,0.0000016497376,0.0000023408686,0.00010117791,0.000057821337,0.0005013028],"genre_scores_gemma":[0.999826,0.000009625437,0.00008242308,0.000002355023,0.0000012425066,0.0000013045609,0.000028175415,0.000005292444,0.0000435847],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999348,0.000011138264,0.0000031358757,0.000017343726,0.000010124565,0.000023435465],"domain_scores_gemma":[0.999464,0.00021242595,0.00009425122,0.00006259294,0.000052109124,0.00011473386],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028494524,0.0003865871,0.00037156817,0.00041644508,0.0004235485,0.0007117162,0.0006718161,0.0002912037,0.001415562],"category_scores_gemma":[0.0015154984,0.00030909947,0.00040831201,0.00021325385,0.0005441404,0.00051445124,0.0005589347,0.0002619879,0.00013282467],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052970345,0.00010062914,0.5240905,0.0000838985,0.00018899626,0.00026937193,0.00047075385,0.43455654,0.02686324,0.0057746796,0.0007503616,0.0063212314],"study_design_scores_gemma":[0.000038022157,0.00006517488,0.22592022,0.000010598482,0.000054326076,0.000045495366,0.00011736223,0.7675006,0.0028599808,0.0030825688,0.0002717278,0.00003397587],"about_ca_topic_score_codex":0.028151063,"about_ca_topic_score_gemma":0.01673651,"teacher_disagreement_score":0.028151063,"about_ca_system_score_codex":0.001061033,"about_ca_system_score_gemma":0.0004477307,"threshold_uncertainty_score":0.055974424},"labels":[],"label_agreement":null},{"id":"W2610346442","doi":"10.3847/1538-4357/aa8d1d","title":"A 2500 deg<sup>2</sup> CMB Lensing Map from Combined South Pole Telescope and Planck Data","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"High Energy Physics; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Gordon and Betty Moore Foundation; University of Illinois at Urbana-Champaign; National Science Foundation; Compute Canada; McGill University; University of Chicago; Canada Research Chairs; National Aeronautics and Space Administration; Argonne National Laboratory; California Institute of Technology; U.S. Department of Energy; University of California, Los Angeles; Ministère de l'Économie, de la Science et de l'Innovation - Québec","keywords":"Physics; South Pole Telescope; Planck; Cosmic microwave background; Telescope; Astronomy; Astrophysics; Gravitational lens; Optics; Anisotropy; Galaxy; Redshift","score_opus":0.020475311902900157,"score_gpt":0.2605762331340283,"score_spread":0.2401009212311281,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2610346442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92191094,0.00039653594,0.0069694677,0.000385891,0.000043746073,0.00004758188,0.05407753,0.0013400431,0.014828215],"genre_scores_gemma":[0.943548,0.00018215725,0.013565105,0.000084904925,0.0000705871,0.00003532104,0.04022233,0.00023711722,0.0020544468],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997702,0.000019641406,0.000009443339,0.00005940356,0.00010359463,0.00003770019],"domain_scores_gemma":[0.9996171,0.00005542385,0.00011464643,0.000051682193,0.00008793702,0.000073195355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034481162,0.00034229556,0.00026157062,0.0019954513,0.00024196372,0.000735338,0.00023265932,0.0002175243,0.0069836644],"category_scores_gemma":[0.00077527796,0.0001835135,0.000601264,0.0022025786,0.00016543463,0.00026117064,0.00056367135,0.00022306836,0.0017720745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010105487,0.00008929886,0.6526925,0.0005046813,0.0008965722,0.0018595542,0.00066269987,0.021537455,0.12447379,0.0043840427,0.047091164,0.14479779],"study_design_scores_gemma":[0.000013834491,0.000021877231,0.97796315,0.00001222902,0.00007398713,0.00027361733,0.00010092398,0.0054351776,0.0046402896,0.0003888412,0.011051414,0.00002462192],"about_ca_topic_score_codex":0.007955053,"about_ca_topic_score_gemma":0.009397073,"teacher_disagreement_score":0.007955053,"about_ca_system_score_codex":0.0004217415,"about_ca_system_score_gemma":0.00030768674,"threshold_uncertainty_score":0.023362696},"labels":[],"label_agreement":null},{"id":"W2611054161","doi":"10.3847/1538-4357/aa71b1","title":"Compact Resolved Ejecta in the Nearest Tidal Disruption Event","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Very Long Baseline Array; Jansky; Physics; Astrophysics; Ejecta; Supermassive black hole; Galaxy; Submillimeter Array; Astronomy; Active galactic nucleus; Star formation; Radio galaxy; Supernova","score_opus":0.025941454702369745,"score_gpt":0.2896339365494912,"score_spread":0.26369248184712146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2611054161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918026,0.000044229513,0.00007802332,0.000031740357,0.0000037167435,0.0000018083653,0.000077530436,0.0000056832587,0.00057700905],"genre_scores_gemma":[0.9996024,0.000009029968,0.000044516928,0.000010739369,0.0000034072714,5.8946836e-7,0.00014961851,0.0000011851305,0.00017849702],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991584,0.0000064983487,0.000005330673,0.000025118261,0.000018196553,0.000028933917],"domain_scores_gemma":[0.9995882,0.000043490592,0.00017226455,0.000028580449,0.000038116374,0.00012933766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012457423,0.00009036308,0.00014344727,0.00050484383,0.00031994822,0.0006136921,0.0001650379,0.00035465907,0.0018473336],"category_scores_gemma":[0.00075408584,0.00009707781,0.00012376411,0.00026770734,0.00023503629,0.00030745743,0.00053623144,0.0002936588,0.0002489924],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003386712,0.0000908534,0.98200005,0.000011622361,0.00004239873,0.002022441,0.00036317282,0.00042852617,0.0076209605,0.0003010711,0.00033835616,0.006441946],"study_design_scores_gemma":[0.000006622113,0.00003862016,0.99749833,0.0000034940806,0.000010255032,0.00072732527,0.00024372544,0.00038175122,0.0004303063,0.00006593084,0.00058913097,0.000004419388],"about_ca_topic_score_codex":0.009139756,"about_ca_topic_score_gemma":0.010358333,"teacher_disagreement_score":0.009139756,"about_ca_system_score_codex":0.00046988062,"about_ca_system_score_gemma":0.000089808986,"threshold_uncertainty_score":0.018173099},"labels":[],"label_agreement":null},{"id":"W2611376115","doi":"10.3847/1538-4357/aa70a0","title":"First Results from BISTRO: A SCUBA-2 Polarimeter Survey of the Gould Belt","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Toronto; Canadian Institute for Theoretical Astrophysics; Western University; University of Manitoba; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Astrophysics Division; National Astronomical Observatory of Japan; National Research Foundation of Korea; National Aeronautics and Space Administration; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; Chinese Academy of Sciences; Academia Sinica; Canadian Institute for Theoretical Astrophysics; National Natural Science Foundation of China; Science and Technology Facilities Council; National Research Foundation; Ministry of Science, ICT and Future Planning","keywords":"James Clerk Maxwell Telescope; Protein filament; Polarimeter; Physics; Magnetic field; Astrophysics; Field (mathematics); Consistency (knowledge bases); Star formation; Polarimetry; Astronomy; Galaxy; Optics; Geometry; Chemistry","score_opus":0.028632069054319035,"score_gpt":0.2637796107013282,"score_spread":0.23514754164700918,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2611376115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928235,0.000078886944,0.0008022378,0.00009570314,0.000006570135,0.00003381798,0.002638119,0.00018695372,0.0033341888],"genre_scores_gemma":[0.98985565,0.000062210565,0.0026802456,0.000102050275,0.000019557081,0.000023540742,0.006509125,0.00004412955,0.00070344383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979883,0.000027834692,0.000009342386,0.000036525467,0.00007409077,0.000053420623],"domain_scores_gemma":[0.99935704,0.000059653154,0.000084000974,0.000116175324,0.00016741424,0.00021570755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028304718,0.00029228654,0.00019403674,0.0012722409,0.00042677642,0.00044385792,0.0002656757,0.00034391668,0.00088095834],"category_scores_gemma":[0.0005470784,0.00014601383,0.00020031464,0.0008390749,0.00028508384,0.0002997132,0.00080898433,0.00027359955,0.00024790558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006469688,0.00024556142,0.8860106,0.00007989748,0.00014579589,0.0007490596,0.0009584484,0.0018129242,0.06832261,0.00039806563,0.0039592427,0.036671],"study_design_scores_gemma":[0.000018907105,0.00005604277,0.994945,0.0000072286534,0.000017909015,0.000089205496,0.00022763613,0.0011890392,0.0017216756,0.00006501434,0.0016496654,0.000012766167],"about_ca_topic_score_codex":0.023217717,"about_ca_topic_score_gemma":0.06436971,"teacher_disagreement_score":0.023217717,"about_ca_system_score_codex":0.00040123347,"about_ca_system_score_gemma":0.00032041862,"threshold_uncertainty_score":0.04616511},"labels":[],"label_agreement":null},{"id":"W2611586798","doi":"10.3847/1538-4357/aa9329","title":"A Mote in Andromeda's Disk: A Misidentified Periodic AGN behind M31","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Comisión Nacional de Investigación Científica y Tecnológica; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Ministério da Ciência, Tecnologia e Inovação; Lawrence Berkeley National Laboratory; Ministerio de Ciencia, Tecnología e Innovación Productiva; Smithsonian Astrophysical Observatory; University System of Taiwan; Weizmann Institute of Science; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University","keywords":"Milky Way; Supermassive black hole; Photometry (optics); Luminosity; Active galactic nucleus; Black hole (networking); Virial mass; Galactic Center; Galaxy","score_opus":0.009738818841198154,"score_gpt":0.23249218632310098,"score_spread":0.22275336748190283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2611586798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986621,0.00006978795,0.0001475783,0.000039942108,0.0000054455013,0.000005118205,0.000054567172,0.000012964672,0.0010024568],"genre_scores_gemma":[0.9995554,0.000014744606,0.00019600318,0.000009553566,0.000004625803,0.0000010434578,0.000047901583,0.0000017978889,0.00016882889],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999316,0.000008443179,0.000004914026,0.000019863994,0.000017371096,0.000017790777],"domain_scores_gemma":[0.99976844,0.00003899509,0.00007619862,0.000030156358,0.000019457433,0.00006679025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013182069,0.00021280312,0.00012516242,0.00086378603,0.00064180134,0.00043083052,0.00030747472,0.00041271254,0.0016549998],"category_scores_gemma":[0.00066482864,0.00010914548,0.00013267936,0.00032345098,0.00021156721,0.000213127,0.0003965937,0.00016329614,0.00039220907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002889877,0.000062925465,0.9098452,0.000041323376,0.00004283727,0.032712605,0.0008681019,0.00072041445,0.03939154,0.00048202276,0.0005269783,0.015017047],"study_design_scores_gemma":[0.00000980129,0.00012452519,0.9763141,0.000017951741,0.000021242278,0.01683805,0.00064393907,0.0018018222,0.0018745889,0.00022018723,0.002121332,0.000012430137],"about_ca_topic_score_codex":0.002772232,"about_ca_topic_score_gemma":0.0051261727,"teacher_disagreement_score":0.002772232,"about_ca_system_score_codex":0.0002651001,"about_ca_system_score_gemma":0.00011430121,"threshold_uncertainty_score":0.0055365562},"labels":[],"label_agreement":null},{"id":"W2611702070","doi":"10.3847/1538-4357/aa72e4","title":"The Disk Physical Conditions of 48 Persei Constrained by Contemporaneous Hα Spectroscopy and Interferometry","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Interferometry; Spectroscopy; RADIUS; Position angle; Very Large Telescope; Observatory; Wavelength; Spectral line; Line (geometry)","score_opus":0.008373945434703487,"score_gpt":0.2686199802973142,"score_spread":0.2602460348626107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2611702070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987239,0.000008618617,0.00048288357,0.000016849668,9.574388e-7,0.0000022853949,0.00014595107,0.00001529772,0.00060318294],"genre_scores_gemma":[0.9991872,0.00001201235,0.00044650983,0.0000045878646,0.0000011822896,0.0000020230668,0.00015920344,0.0000059378513,0.00018141886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999378,0.000008455318,0.000002525957,0.000026009142,0.000013159665,0.000012154659],"domain_scores_gemma":[0.99984694,0.000019717276,0.00004713016,0.000045710705,0.000019318324,0.000021259824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001409359,0.00028721313,0.00023787693,0.000264351,0.00027992338,0.00045468158,0.00031994242,0.0002644657,0.00088465185],"category_scores_gemma":[0.00057899475,0.00023848758,0.0001855165,0.00023768467,0.00023691608,0.00049807515,0.00025222063,0.0002205603,0.00031165048],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045366448,0.00022303067,0.7195404,0.000030891755,0.00010883867,0.0009906922,0.00036064856,0.20655343,0.04916167,0.0029878619,0.001399017,0.018189762],"study_design_scores_gemma":[0.000055407298,0.00016037114,0.50359714,0.000009759909,0.00004235951,0.00045059735,0.00043880992,0.47687858,0.01205061,0.0029391944,0.0033338517,0.000043313157],"about_ca_topic_score_codex":0.008396335,"about_ca_topic_score_gemma":0.009006369,"teacher_disagreement_score":0.008396335,"about_ca_system_score_codex":0.0005963265,"about_ca_system_score_gemma":0.00023334734,"threshold_uncertainty_score":0.016694903},"labels":[],"label_agreement":null},{"id":"W2611779013","doi":"10.3847/1538-4357/aa706b","title":"Discovery of a Rapid, Luminous Nova in NGC 300 by the KMTNet Supernova Program","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Nova (rocket); Supernova; Physics; Astrophysics; Astronomy; Aeronautics; Engineering","score_opus":0.016291750396905575,"score_gpt":0.26304379076939893,"score_spread":0.24675204037249335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2611779013","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949516,0.00021466779,0.00069098826,0.00009421224,0.000021684275,0.000019134535,0.00039987577,0.000057820762,0.0035500675],"genre_scores_gemma":[0.99831307,0.00008081947,0.0005937599,0.00004741947,0.000011193391,0.0000046407067,0.00055392715,0.000009209874,0.00038588652],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998795,0.0000076130123,0.000010883328,0.000034644654,0.00004148906,0.000025884301],"domain_scores_gemma":[0.9994942,0.00003327882,0.00012832042,0.0000511776,0.000046267975,0.00024676428],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043627573,0.00018040689,0.00015792552,0.0007731215,0.0004943551,0.0006995795,0.00023401286,0.00022548084,0.0006497957],"category_scores_gemma":[0.00037663232,0.000099024226,0.00027365852,0.0003453426,0.00026905836,0.00021328454,0.00059597223,0.00028127898,0.00016130153],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025362807,0.000080779166,0.93391454,0.000045364286,0.00007521717,0.004142776,0.00027397956,0.0007434299,0.041781202,0.0017181778,0.0011606801,0.015810303],"study_design_scores_gemma":[0.000011444437,0.00013465328,0.98518974,0.00003177434,0.00002991734,0.0029036843,0.00022077565,0.0012715041,0.0059212367,0.00050897495,0.0037616158,0.0000145795475],"about_ca_topic_score_codex":0.0037970338,"about_ca_topic_score_gemma":0.010888926,"teacher_disagreement_score":0.0037970338,"about_ca_system_score_codex":0.0006039031,"about_ca_system_score_gemma":0.00028140075,"threshold_uncertainty_score":0.0075498223},"labels":[],"label_agreement":null},{"id":"W2612357861","doi":"10.3847/1538-4357/aa960f","title":"Deep Submillimeter and Radio Observations in the SSA22 Field. I. Powering Sources and the Lyα Escape Fraction of Lyα Blobs","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; Knut och Alice Wallenbergs Stiftelse; Chinese Academy of Sciences; Academia Sinica; Youth Innovation Promotion Association; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Natural Science Foundation of China; National Radio Astronomy Observatory; Youth Innovation Promotion Association of the Chinese Academy of Sciences; Vetenskapsrådet; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Extinction (optical mineralogy); Attenuation; Fraction (chemistry); Cosmic dust; Star formation; Absorption (acoustics); Optical depth; Radio astronomy","score_opus":0.01088897839713147,"score_gpt":0.21879406414563213,"score_spread":0.20790508574850067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2612357861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99934036,0.00008749989,0.000049894414,0.000005713784,9.750619e-7,0.0000015774301,0.00023915585,0.0000058204914,0.00026899247],"genre_scores_gemma":[0.9988618,0.000064307416,0.00006814061,0.000008210517,0.0000067514293,0.0000030850044,0.0006423447,0.000003121298,0.00034223328],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990654,0.000009707829,0.0000047213744,0.00002645582,0.000016920781,0.000035557885],"domain_scores_gemma":[0.99939215,0.000050486084,0.00022578031,0.00003749314,0.00007797217,0.00021620716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018063135,0.0003302648,0.0002809359,0.0014767402,0.00026891578,0.0005090005,0.00015496937,0.00018612955,0.0013020217],"category_scores_gemma":[0.00030830016,0.00013190255,0.00018590785,0.0008561376,0.00025910363,0.00026958887,0.0004252653,0.00015454144,0.00047762413],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000090152,0.000034590495,0.98475766,0.000016280117,0.000031633503,0.00016554835,0.00046245262,0.00008844608,0.009563139,0.000027358612,0.00016571801,0.004596915],"study_design_scores_gemma":[8.567959e-7,0.0000123624,0.99965394,0.0000011623633,0.0000025054042,0.000025363073,0.000084713625,0.000027153756,0.00007814515,0.000004058679,0.00010895624,7.6396736e-7],"about_ca_topic_score_codex":0.011602671,"about_ca_topic_score_gemma":0.02024098,"teacher_disagreement_score":0.011602671,"about_ca_system_score_codex":0.00030164674,"about_ca_system_score_gemma":0.00009462507,"threshold_uncertainty_score":0.023070276},"labels":[],"label_agreement":null},{"id":"W2612904700","doi":"10.3847/1538-4357/aa8b6c","title":"Next Generation Virgo Cluster Survey. XXI. The Weak Lensing Masses of the CFHTLS and NGVS RedGOLD Galaxy Clusters and Calibration of the Optical Richness","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Galaxy cluster; Cluster (spacecraft); Weak gravitational lensing; Redshift; Galaxy; Halo; Virgo Cluster; Gravitational lens","score_opus":0.02152587941454978,"score_gpt":0.2298663704028543,"score_spread":0.2083404909883045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2612904700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898617,0.00008961606,0.0010496802,0.000024481824,0.000003577904,0.000013803358,0.0068724724,0.00007642465,0.0020082602],"genre_scores_gemma":[0.99068975,0.000024234956,0.0015135406,0.000010171562,0.000003252273,0.000009359283,0.0072416696,0.000016274864,0.0004917429],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972314,0.000066732086,0.000013738859,0.00007641319,0.00005899693,0.00006103338],"domain_scores_gemma":[0.9994405,0.00008640786,0.00017092351,0.00013167635,0.00007981573,0.000090652386],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008957338,0.0002486119,0.0001272637,0.0010015081,0.00020373038,0.00028860013,0.0002959416,0.00011881188,0.0011493104],"category_scores_gemma":[0.0012148607,0.00011779154,0.0002340144,0.00071811496,0.00014198951,0.00020729406,0.00043807813,0.00011769251,0.00038878596],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000545453,0.000009341849,0.98993146,0.000014865256,0.000057999583,0.000021407948,0.000064970074,0.002031917,0.0012967797,0.0004131765,0.00086045894,0.00524307],"study_design_scores_gemma":[0.0000037187992,0.0000075447915,0.9945104,0.0000028232375,0.000012718736,0.000024716746,0.000036699836,0.003214149,0.0009664174,0.00008233496,0.0011339302,0.000004425066],"about_ca_topic_score_codex":0.051954795,"about_ca_topic_score_gemma":0.08633192,"teacher_disagreement_score":0.051954795,"about_ca_system_score_codex":0.00068545446,"about_ca_system_score_gemma":0.00026608715,"threshold_uncertainty_score":0.1033048},"labels":[],"label_agreement":null},{"id":"W2613196871","doi":"10.3847/1538-4357/aa86a9","title":"The Mira-Titan Universe. II. Matter Power Spectrum Emulation","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":133,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"Oak Ridge National Laboratory; Argonne National Laboratory; Aspen Center for Physics; Advanced Scientific Computing Research; High Energy Physics; U.S. Department of Energy; Office of Science; National Science Foundation","keywords":"Matter power spectrum; Physics; Neutrino; Dark energy; COSMIC cancer database; Redshift; Spectral density; Cosmology; Universe; Computer science; Astrophysics; Particle physics","score_opus":0.0061343102770903945,"score_gpt":0.21046214091543133,"score_spread":0.20432783063834095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2613196871","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.40777576,0.00040390767,0.5076708,0.0007148072,0.00023431958,0.00028419483,0.015002588,0.02178546,0.046128247],"genre_scores_gemma":[0.7942526,0.00014944989,0.18747734,0.00025284922,0.000054793563,0.00032233185,0.010651061,0.0024300078,0.004409685],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99974006,0.000090066,0.000010962024,0.000044678098,0.00008615009,0.000028034694],"domain_scores_gemma":[0.99942374,0.0001398037,0.000042881657,0.00024206577,0.00011851935,0.00003294765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007477183,0.0004912138,0.00037305534,0.00046537296,0.0003773385,0.00070813985,0.0013618317,0.0005273218,0.0037192802],"category_scores_gemma":[0.0036037208,0.0003126349,0.00048604017,0.00054516,0.00029649824,0.001010802,0.00061508454,0.000752013,0.0011981894],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031576428,0.00012307495,0.022137266,0.00014018331,0.00014620656,0.00024089756,0.00024565775,0.85374635,0.006291361,0.06413709,0.014523959,0.037952203],"study_design_scores_gemma":[0.000028479373,0.000022545159,0.0024683883,0.000010681201,0.000007844154,0.000060312974,0.000013582545,0.9784323,0.0037835536,0.008053969,0.007104451,0.000013910852],"about_ca_topic_score_codex":0.006164234,"about_ca_topic_score_gemma":0.0035684265,"teacher_disagreement_score":0.006164234,"about_ca_system_score_codex":0.0006485599,"about_ca_system_score_gemma":0.0005225694,"threshold_uncertainty_score":0.012442172},"labels":[],"label_agreement":null},{"id":"W2613328227","doi":"10.3847/1538-4357/aa8e9f","title":"A Measurement of the Cosmic Microwave Background B-mode Polarization Power Spectrum at Subdegree Scales from Two Years of polarbear Data","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Dalhousie University","funders":"Los Alamos National Laboratory; Japan Society for the Promotion of Science; Comisión Nacional de Investigación Científica y Tecnológica; McGill University; University of California, Irvine; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; European Commission; Ministry of Education, Culture, Sports, Science and Technology; Centre National d’Etudes Spatiales; Office of Science; National Aeronautics and Space Administration; National Science Foundation","keywords":"Cosmic microwave background; Gravitational lens; Polarization (electrochemistry); Amplitude; Spectral density; COSMIC cancer database; Weak gravitational lensing; Observational cosmology; Cosmic infrared background; Cosmic background radiation","score_opus":0.02669986263360764,"score_gpt":0.27788856558318686,"score_spread":0.25118870294957923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2613328227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900538,0.000099047575,0.0035855162,0.00006288328,0.000015494312,0.000014416127,0.0045064283,0.00011879838,0.001543604],"genre_scores_gemma":[0.98436534,0.000076215416,0.0042814794,0.000041349933,0.000043549335,0.0000363801,0.010851525,0.00004661204,0.00025753118],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954563,0.00010989224,0.000023101433,0.00014358357,0.000102012425,0.00007571743],"domain_scores_gemma":[0.99795014,0.00047082783,0.00049487903,0.00046797088,0.00035899295,0.00025719247],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011049338,0.00039186896,0.00025862164,0.001844308,0.00034557955,0.0006637988,0.00033092228,0.00033840808,0.0009965659],"category_scores_gemma":[0.0017347663,0.0002895849,0.00040150018,0.0015089443,0.00022554124,0.00046960995,0.00066955143,0.00046312137,0.00040519892],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009116786,0.00025842176,0.8877255,0.00012413954,0.0005453958,0.0003339172,0.00032429167,0.0067623327,0.07278755,0.0010260117,0.002439954,0.02676093],"study_design_scores_gemma":[0.000019787123,0.000050716375,0.98489517,0.0000096060785,0.00006315193,0.00011289658,0.00004215082,0.0037301274,0.008282518,0.00018732778,0.0025862094,0.000020426356],"about_ca_topic_score_codex":0.0034909304,"about_ca_topic_score_gemma":0.005745505,"teacher_disagreement_score":0.0034909304,"about_ca_system_score_codex":0.0002524795,"about_ca_system_score_gemma":0.00016649158,"threshold_uncertainty_score":0.0069411993},"labels":[],"label_agreement":null},{"id":"W2613468866","doi":"10.3847/1538-4357/aa61fe","title":"The Mass, Color, and Structural Evolution of Today’s Massive Galaxies Since z ∼ 5","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Stellar mass; Astronomy; Galaxy formation and evolution; Star formation","score_opus":0.006067154144475308,"score_gpt":0.2176817254754547,"score_spread":0.21161457133097938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2613468866","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986772,0.00004352881,0.00039152004,0.000011603814,0.0000012512949,9.204113e-7,0.0002270479,0.000029226283,0.0006176837],"genre_scores_gemma":[0.99918216,0.000015442482,0.0003367748,0.0000034419986,0.000001783126,3.9833046e-7,0.00033436995,0.0000032532607,0.00012234016],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994874,0.0000040925147,0.000002025841,0.000015139888,0.000012537685,0.00001748218],"domain_scores_gemma":[0.99956685,0.000050686212,0.00018617958,0.00004079087,0.000054999426,0.00010053716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023762963,0.00013125289,0.00008441044,0.0010057747,0.00021472246,0.00050292816,0.00019905971,0.00010905476,0.0009636314],"category_scores_gemma":[0.0005744349,0.00008925915,0.00019480291,0.00040582768,0.00016450169,0.0002767475,0.00030566612,0.00017678425,0.00024397935],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033356464,0.000012962137,0.98405623,0.0000059783288,0.000036102138,0.000059337144,0.00017983472,0.0013639164,0.0057347417,0.00056308095,0.00025073934,0.007703788],"study_design_scores_gemma":[5.274634e-7,0.00001200397,0.99607724,0.0000016664613,0.000007845032,0.000031545882,0.000049827482,0.0024456207,0.00094775885,0.00009195872,0.00033197628,0.0000019295721],"about_ca_topic_score_codex":0.0074906317,"about_ca_topic_score_gemma":0.008920864,"teacher_disagreement_score":0.0074906317,"about_ca_system_score_codex":0.0002544903,"about_ca_system_score_gemma":0.00009515496,"threshold_uncertainty_score":0.014894068},"labels":[],"label_agreement":null},{"id":"W2613683462","doi":"10.3847/1538-4357/aa6caf","title":"An ALMA Survey of Submillimeter Galaxies in the Extended Chandra Deep Field South: Spectroscopic Redshifts","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Photometry (optics); Star formation; Astronomy; Chandra Deep Field South; Photometric redshift; Stellar mass; Submillimeter Array; Spectral density; Luminous infrared galaxy; Stars","score_opus":0.016479689440468535,"score_gpt":0.25574744852020115,"score_spread":0.2392677590797326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2613683462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99440324,0.0002074992,0.0006298763,0.00004281555,0.0000062143017,0.000018937872,0.0033960599,0.00013402305,0.0011613915],"genre_scores_gemma":[0.9917794,0.00012715181,0.0019772304,0.0000654755,0.00002790402,0.000021854044,0.0054395804,0.000033142376,0.0005284223],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997105,0.0000473384,0.00001760865,0.00008147236,0.000076477685,0.000066537104],"domain_scores_gemma":[0.9984799,0.0002014372,0.0004307535,0.00030748037,0.00021022302,0.00037027575],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074229314,0.00029087102,0.00024264012,0.0027796163,0.00029089238,0.00046604127,0.00037117573,0.00013255997,0.0017244952],"category_scores_gemma":[0.0011496881,0.00017868365,0.00033995765,0.0014999798,0.00015311848,0.00034798615,0.0006429257,0.00020353291,0.0006219272],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013086096,0.000065196255,0.9667654,0.000037701942,0.00007569723,0.00005459151,0.00018301245,0.00047076333,0.0084403185,0.00031011543,0.0025633236,0.020903],"study_design_scores_gemma":[0.00000950187,0.000019969792,0.99665654,0.000005537003,0.0000125944525,0.00005467276,0.000036370864,0.00060924265,0.0006521432,0.000069055925,0.0018689837,0.0000053052167],"about_ca_topic_score_codex":0.007304908,"about_ca_topic_score_gemma":0.013115883,"teacher_disagreement_score":0.007304908,"about_ca_system_score_codex":0.00026279798,"about_ca_system_score_gemma":0.00025163262,"threshold_uncertainty_score":0.014524758},"labels":[],"label_agreement":null},{"id":"W2613903437","doi":"10.3847/1538-4357/aa8508","title":"Search for Astrophysical Sources of Neutrinos Using Cascade Events in IceCube","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Science and Technology Facilities Council","keywords":"Physics; Neutrino; Sky; Muon neutrino; Cascade; Astrophysics; Flux (metallurgy); Muon; Neutrino detector; Cosmic neutrino background; Solar neutrino; Observatory; Astronomy; Particle physics; Neutrino oscillation","score_opus":0.02764364713591136,"score_gpt":0.29131888525508154,"score_spread":0.26367523811917015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2613903437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927636,0.00010545018,0.0012852477,0.000020305177,0.0000053114904,0.0000719448,0.0028537007,0.00004269545,0.0028518098],"genre_scores_gemma":[0.98810065,0.00012885095,0.0036177146,0.000023234737,0.000019727888,0.000057727255,0.007448491,0.000029727773,0.00057389366],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996088,0.00008139155,0.000015909656,0.00011926679,0.00010186487,0.00007271218],"domain_scores_gemma":[0.99923956,0.00020509279,0.00024276134,0.000084021856,0.00011970306,0.00010881722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007436239,0.0004160685,0.00038934918,0.0016174567,0.00057797297,0.0006935149,0.0003009797,0.00018869307,0.0017475105],"category_scores_gemma":[0.00085635914,0.00021263176,0.00044123002,0.0014138664,0.00027064682,0.00028565788,0.0007323432,0.00021386247,0.00023005003],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013270654,0.00014730399,0.9388428,0.000056543988,0.0002921201,0.00071305706,0.00031897033,0.0026471766,0.04298415,0.0006645545,0.001227679,0.010778692],"study_design_scores_gemma":[0.00004972189,0.00018043377,0.979518,0.000016484797,0.000103548504,0.000526103,0.00022851399,0.0053607235,0.01053753,0.0002969977,0.0031667945,0.000015231078],"about_ca_topic_score_codex":0.008332334,"about_ca_topic_score_gemma":0.018965855,"teacher_disagreement_score":0.008332334,"about_ca_system_score_codex":0.00051257684,"about_ca_system_score_gemma":0.0005155833,"threshold_uncertainty_score":0.016567707},"labels":[],"label_agreement":null},{"id":"W2613923715","doi":"10.3847/1538-4357/aa713d","title":"On a New Theoretical Framework for RR Lyrae Stars. II. Mid-infrared Period–Luminosity–Metallicity Relations","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"European Space Agency; California Institute of Technology; University of California, Los Angeles; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"RR Lyrae variable; Metallicity; Physics; Astrophysics; Globular cluster; Distance modulus; Luminosity; Stars; Wavelength; Astronomy; Galaxy; Optics","score_opus":0.015596265229605017,"score_gpt":0.2596164188048531,"score_spread":0.24402015357524806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2613923715","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.097219266,0.004524672,0.7942101,0.0059101046,0.00042227723,0.0000746516,0.0003202541,0.00047620837,0.096842416],"genre_scores_gemma":[0.862842,0.0026722534,0.11750237,0.00081202685,0.0013171688,0.0002567381,0.00030918038,0.00021792989,0.014070229],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9995117,0.0001298887,0.000021785072,0.000119973876,0.00015100063,0.00006568059],"domain_scores_gemma":[0.99908316,0.00038150288,0.00016138157,0.00014526013,0.000174241,0.000054494678],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020319596,0.0006205518,0.00042320363,0.0023926059,0.001072265,0.0015822606,0.0019127285,0.0011649977,0.004792198],"category_scores_gemma":[0.0027715073,0.00034214454,0.0012024598,0.00085491966,0.0028236853,0.0035863349,0.0013283556,0.0013875293,0.0013636285],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00000484748,0.00001442827,0.0013056374,0.000035999867,0.000008048829,0.00006630892,0.00017778763,0.021999953,0.00048156726,0.96531403,0.0013355205,0.00925592],"study_design_scores_gemma":[0.000008875891,0.000023998844,0.0017567889,0.00002350111,0.000005383777,0.0001253539,0.00005466351,0.11203339,0.00017859609,0.87434065,0.011431583,0.000017137254],"about_ca_topic_score_codex":0.0020281447,"about_ca_topic_score_gemma":0.0011601577,"teacher_disagreement_score":0.004792198,"about_ca_system_score_codex":0.0018890736,"about_ca_system_score_gemma":0.00056817447,"threshold_uncertainty_score":0.016031444},"labels":[],"label_agreement":null},{"id":"W2614400323","doi":"10.3847/1538-4357/aa72dd","title":"Improving and Assessing Planet Sensitivity of the GPI Exoplanet Survey with a Forward Model Matched Filter","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Université de Montréal; Western University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Exoplanet; Planet; False positive paradox; Matched filter; Physics; Sensitivity (control systems); Astrophysics; False positive rate; Stars; Computer science; Point spread function; Light curve; Algorithm; Filter (signal processing); Artificial intelligence; Optics; Computer vision","score_opus":0.020028483944984257,"score_gpt":0.2374058554894823,"score_spread":0.21737737154449804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2614400323","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8249088,0.00015817392,0.17075284,0.00007427807,0.000009950729,0.000057527413,0.00061100966,0.0017244307,0.0017030397],"genre_scores_gemma":[0.894346,0.000041765274,0.104183055,0.000022710721,0.000008090818,0.000029307344,0.0009021794,0.00006484606,0.0004019514],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991959,0.00018506059,0.00004158072,0.00021146981,0.00030674777,0.000059268285],"domain_scores_gemma":[0.9984915,0.00057327654,0.00020395561,0.0003718701,0.00029304586,0.00006634964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016230621,0.00036165453,0.00027732595,0.00156492,0.0002266778,0.00055751356,0.00045884663,0.00042333113,0.0006385305],"category_scores_gemma":[0.0038354609,0.00024277804,0.00043823686,0.00064653746,0.00015809592,0.00047275753,0.0007836792,0.00021353991,0.00030612544],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008005299,0.00021908856,0.4484278,0.00014741259,0.0003928544,0.00020073938,0.00019535897,0.10189244,0.113918,0.0013487092,0.001648156,0.33080888],"study_design_scores_gemma":[0.00003633753,0.0002884456,0.3871958,0.0000150072265,0.00013752539,0.0004661791,0.000072725365,0.54596055,0.06216146,0.000841198,0.002781545,0.000043188036],"about_ca_topic_score_codex":0.001904302,"about_ca_topic_score_gemma":0.0026317479,"teacher_disagreement_score":0.001904302,"about_ca_system_score_codex":0.0003378507,"about_ca_system_score_gemma":0.00022478298,"threshold_uncertainty_score":0.008583665},"labels":[],"label_agreement":null},{"id":"W2615272527","doi":"10.3847/1538-4357/aa8628","title":"Greatly Enhanced Merger Rates of Compact-object Binaries in Non-spherical Nuclear Star Clusters","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":180,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Eccentricity (behavior); Neutron star; Compact star; Star cluster; Precession; Cluster (spacecraft); Gravitational wave; X-ray binary; Orbital eccentricity; Binary number; Galaxy; Stars; Astronomy","score_opus":0.016338171270150307,"score_gpt":0.3309976144880011,"score_spread":0.3146594432178508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2615272527","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998022,0.000018660072,0.000059999533,0.0000028591953,6.2571314e-7,6.566892e-7,0.000009099772,0.0000041057488,0.00010174912],"genre_scores_gemma":[0.99990165,0.0000059420913,0.000028549633,7.503764e-7,5.2950975e-7,3.5103454e-7,0.000025623669,8.348388e-7,0.000035820874],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982846,0.000026543568,0.000010521573,0.000048957936,0.000039885505,0.000045538647],"domain_scores_gemma":[0.9994087,0.00012832475,0.00019593442,0.00007017073,0.00006681513,0.00012997653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003690492,0.00016287892,0.00022816117,0.00042628488,0.000323988,0.0004935598,0.0003242386,0.00020536374,0.0006946669],"category_scores_gemma":[0.0013802325,0.00013045619,0.00012522307,0.0002512553,0.00032120864,0.0002677908,0.00065322354,0.00014855435,0.00013516677],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010583729,0.00011599595,0.83867127,0.00007201555,0.00016065816,0.00093817,0.00058596383,0.030146703,0.116297714,0.0023880003,0.0004157599,0.009149358],"study_design_scores_gemma":[0.000022727829,0.00020266214,0.9245683,0.0000048780244,0.000044256212,0.00056221266,0.00038983987,0.045551643,0.027651755,0.00046269377,0.0005135101,0.000025584966],"about_ca_topic_score_codex":0.0019100651,"about_ca_topic_score_gemma":0.0017034748,"teacher_disagreement_score":0.0019100651,"about_ca_system_score_codex":0.00047634487,"about_ca_system_score_gemma":0.0001425059,"threshold_uncertainty_score":0.0037979484},"labels":[],"label_agreement":null},{"id":"W2615313038","doi":"10.3847/1538-4357/aa73de","title":"Spin-down Evolution and Radio Disappearance of the Magnetar PSR J1622–4950","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Magnetar; Pulsar; Neutron star; Flux (metallurgy); Pulse (music); Luminosity; Magnitude (astronomy); Magnetic flux","score_opus":0.009397461122769056,"score_gpt":0.30000500148737624,"score_spread":0.2906075403646072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2615313038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998808,0.00017251582,0.00009530463,0.000018312316,0.000007713483,0.0000033686817,0.00021688927,0.0000101070045,0.000667681],"genre_scores_gemma":[0.99900764,0.00005200884,0.00008364607,0.000013846366,0.00001233663,0.000003927745,0.0004827343,0.000005359429,0.00033846192],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998518,0.00001606963,0.00001027472,0.000043300864,0.000041736697,0.000036862162],"domain_scores_gemma":[0.99945265,0.000038599665,0.00021823637,0.000065669956,0.00009593856,0.00012892263],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034726586,0.00033296153,0.00035099615,0.0009093228,0.000374421,0.00058347976,0.00031597086,0.0003107835,0.001126531],"category_scores_gemma":[0.00083610066,0.00021419939,0.00019065657,0.00042562647,0.0003471851,0.00032878263,0.0005648373,0.00032734827,0.0005591649],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003740654,0.00008539498,0.93316454,0.000029519711,0.00012023274,0.0006506794,0.00023000731,0.00037858164,0.05463558,0.000118290736,0.00041623233,0.009796753],"study_design_scores_gemma":[0.0000053070607,0.00007517236,0.9979627,0.0000035967391,0.000010826268,0.00013043084,0.000053991622,0.00015184059,0.000929458,0.000013707604,0.00065845303,0.000004527061],"about_ca_topic_score_codex":0.0056770905,"about_ca_topic_score_gemma":0.0089579215,"teacher_disagreement_score":0.0056770905,"about_ca_system_score_codex":0.00039622356,"about_ca_system_score_gemma":0.00016643935,"threshold_uncertainty_score":0.011288106},"labels":[],"label_agreement":null},{"id":"W2615662771","doi":"10.1088/0004-637x/704/2/1002","title":"ANISOTROPIC ACTIVE GALACTIC NUCLEUS OUTFLOWS AND ENRICHMENT OF THE INTERGALACTIC MEDIUM. I. METAL DISTRIBUTION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Active galactic nucleus; Redshift; Anisotropy; Intergalactic travel; Kinetic energy; Volume fraction; Quasar; Cosmology","score_opus":0.005503301485910498,"score_gpt":0.21128725029946177,"score_spread":0.20578394881355128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2615662771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974904,0.00006455918,0.0015379669,0.00002896148,0.0000025741695,0.0000044440603,0.00007247849,0.000023490298,0.00077520206],"genre_scores_gemma":[0.99902296,0.000036040972,0.0006966715,0.000008931467,0.000002423622,0.0000032103826,0.00007107763,0.000009020198,0.00014968387],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.999889,0.000033539705,0.0000056416643,0.000022211732,0.000014281819,0.00003528375],"domain_scores_gemma":[0.99944824,0.0001903287,0.00018345375,0.00004993617,0.000045302495,0.000082743914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025944653,0.00039386383,0.00024069038,0.0004283403,0.00024451918,0.0005663281,0.0005125329,0.0004905272,0.00076029013],"category_scores_gemma":[0.0015425597,0.00023747899,0.0004721439,0.00039254423,0.00048280184,0.0004432603,0.0005064409,0.00032434092,0.000071804505],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022928351,0.000094954616,0.10851319,0.000046103803,0.000082356346,0.0002923779,0.0001015126,0.8668736,0.017835433,0.0034485448,0.00016571612,0.0023169597],"study_design_scores_gemma":[0.00004028434,0.000057520592,0.032226652,0.000007475485,0.000026702508,0.000051227198,0.0000537029,0.9615633,0.0046158377,0.001108333,0.00023553795,0.000013397636],"about_ca_topic_score_codex":0.011102013,"about_ca_topic_score_gemma":0.0065595154,"teacher_disagreement_score":0.011102013,"about_ca_system_score_codex":0.0007931836,"about_ca_system_score_gemma":0.0002670094,"threshold_uncertainty_score":0.022074819},"labels":[],"label_agreement":null},{"id":"W2615830046","doi":"10.3847/1538-4357/aa75ca","title":"Asteroseismology and Gaia: Testing Scaling Relations Using 2200 Kepler Stars with TGAS Parallaxes","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":277,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Centre National d’Etudes Spatiales; University of Oxford; York University; Villum Fonden; Leibniz-Gemeinschaft; University of Notre Dame; Ohio State University; National Research Foundation; Carnegie Mellon University; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; Stellar Astrophysics Centre; University of Utah; Carnegie Institution of Washington; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; National Science Foundation","keywords":"Asteroseismology; Parallax; Stars; Scaling; Photometry (optics); Metallicity; Kepler; Giant star; Infrared","score_opus":0.033322022149283814,"score_gpt":0.25633144714683975,"score_spread":0.22300942499755594,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2615830046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984829,0.000025822967,0.00037672746,0.000008338629,0.0000029776822,0.000003913321,0.0003704803,0.000027095162,0.00070168707],"genre_scores_gemma":[0.99888736,0.000007647942,0.00036923596,0.000003598973,0.0000026294717,0.0000033997467,0.0006145043,0.000010008223,0.00010163712],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990238,0.00025460988,0.00008603125,0.00036176422,0.00020674859,0.00006712093],"domain_scores_gemma":[0.99191964,0.0035237246,0.0014568075,0.0013493423,0.0010507521,0.0006997409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014595358,0.00038402987,0.00025502368,0.0016538627,0.0002883402,0.00084175594,0.00036637887,0.0003377103,0.0010509794],"category_scores_gemma":[0.0107157435,0.0001506869,0.00041936216,0.0010781232,0.00036786599,0.0008218298,0.0009359015,0.00029938304,0.0008815037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023463712,0.0000399147,0.9868787,0.00001353837,0.000086767075,0.00005484928,0.0002549064,0.0021038936,0.0024559284,0.0001937061,0.0001630816,0.0075200433],"study_design_scores_gemma":[0.000013437642,0.00023367406,0.9866173,0.000005369987,0.000017056069,0.00013286137,0.00030824277,0.009703874,0.002038541,0.00019138443,0.0007304227,0.000007829859],"about_ca_topic_score_codex":0.0028959352,"about_ca_topic_score_gemma":0.0019413631,"teacher_disagreement_score":0.0028959352,"about_ca_system_score_codex":0.00037357278,"about_ca_system_score_gemma":0.00013235018,"threshold_uncertainty_score":0.007718861},"labels":[],"label_agreement":null},{"id":"W2617164508","doi":"10.3847/1538-4357/aa9700","title":"A Multi-telescope Campaign on FRB 121102: Implications for the FRB Population","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":188,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Telescope; Population; Astronomy; Astrophysics; Medicine","score_opus":0.03278574415815867,"score_gpt":0.29907591462137856,"score_spread":0.2662901704632199,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2617164508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965322,0.00011741019,0.00071814447,0.000093538765,0.000011342586,0.000010169657,0.0011573016,0.00005839968,0.0013015245],"genre_scores_gemma":[0.99655366,0.00003570203,0.00046997753,0.00003943034,0.000019240373,0.000011682059,0.002448025,0.00002873404,0.0003934383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99877554,0.00020578163,0.00004583913,0.00040886315,0.0003012913,0.00026255567],"domain_scores_gemma":[0.99467635,0.00088954956,0.0019507855,0.0007659454,0.0006794455,0.0010379442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017025652,0.000435341,0.0005121912,0.0016645549,0.0008907312,0.00092709955,0.00056614,0.0006287582,0.0015572306],"category_scores_gemma":[0.0024727338,0.00026148907,0.00043799588,0.0013274229,0.00039323297,0.00048945687,0.0007846828,0.0005186647,0.00055105134],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059523113,0.00017650174,0.9511328,0.000034489913,0.0001259641,0.00043001794,0.0003721658,0.0017137367,0.030094929,0.00031459343,0.0011215468,0.013888008],"study_design_scores_gemma":[0.000007981797,0.000058831945,0.99773777,0.0000032705414,0.000012755265,0.00012634302,0.00006780458,0.00067389273,0.0007079797,0.00003666224,0.00055997475,0.0000067301603],"about_ca_topic_score_codex":0.013669142,"about_ca_topic_score_gemma":0.017366182,"teacher_disagreement_score":0.013669142,"about_ca_system_score_codex":0.0011385222,"about_ca_system_score_gemma":0.00023314319,"threshold_uncertainty_score":0.027179122},"labels":[],"label_agreement":null},{"id":"W2617363210","doi":"10.3847/1538-4357/aa756a","title":"Galaxy Merger Candidates in High-redshift Cluster Environments","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; York University; McGill University","funders":"","keywords":"Cluster (spacecraft); Galaxy cluster; Brightest cluster galaxy; Galaxy; Galaxy merger; Galaxy groups and clusters; Type-cD galaxy","score_opus":0.006239402107917353,"score_gpt":0.21134312567213673,"score_spread":0.20510372356421938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2617363210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994499,0.000080320446,0.000051474744,0.000008120561,6.777018e-7,0.0000021789572,0.00011083302,0.000007106878,0.0002893529],"genre_scores_gemma":[0.9995578,0.00002084669,0.000066302346,0.0000039969264,0.0000018961684,0.0000013933005,0.00027014632,0.000001945759,0.00007554863],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996469,0.000052977288,0.00002192672,0.00010486063,0.00007472029,0.00009859326],"domain_scores_gemma":[0.9988164,0.00019106959,0.00045253977,0.000092358656,0.00013940144,0.00030825735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032835503,0.00019916812,0.00028412326,0.0026799683,0.0006313921,0.00089208165,0.00029592693,0.00023690707,0.0025623888],"category_scores_gemma":[0.0013347372,0.00013509502,0.00016656716,0.0015228398,0.0003805108,0.00038143407,0.0010210255,0.00014053423,0.00036805857],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017995176,0.000019954123,0.9942509,0.000010788409,0.00003767317,0.00012593488,0.00019914172,0.00015144791,0.0026777077,0.00011530573,0.00016232097,0.0020688723],"study_design_scores_gemma":[0.000002740204,0.000016788139,0.9990238,0.0000018808466,0.000014887998,0.0001594991,0.00016692198,0.00017807179,0.00024802072,0.000030342535,0.00015489198,0.0000020177347],"about_ca_topic_score_codex":0.0045335055,"about_ca_topic_score_gemma":0.0069336267,"teacher_disagreement_score":0.0045335055,"about_ca_system_score_codex":0.00030140154,"about_ca_system_score_gemma":0.00018775946,"threshold_uncertainty_score":0.009014249},"labels":[],"label_agreement":null},{"id":"W2617573518","doi":"10.3847/1538-4357/aa74b1","title":"The Spectroscopy and H-band Imaging of Virgo Cluster Galaxies (SHIVir) Survey: Scaling Relations and the Stellar-to-total Mass Relation","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Herzberg Institute of Astrophysics; Queen's University","funders":"","keywords":"Virgo Cluster; Galaxy; Fundamental plane (elliptical galaxies); Dark matter; Scaling; Galaxy cluster; Galaxy formation and evolution; Tully–Fisher relation; Halo; Mass distribution","score_opus":0.00648549972393569,"score_gpt":0.22364773643527316,"score_spread":0.21716223671133747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2617573518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99813384,0.00013232937,0.00035519956,0.00001472073,0.000001095203,0.0000026631799,0.00038158044,0.00002310242,0.0009555313],"genre_scores_gemma":[0.9993942,0.000023924777,0.00015496065,0.0000058588043,0.0000019261563,0.000001734858,0.0003463486,0.0000038442763,0.000067176166],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978215,0.00004607924,0.000011474778,0.00007353926,0.000042914216,0.000043929598],"domain_scores_gemma":[0.9991886,0.00017480466,0.00022944444,0.00013888613,0.00012523287,0.00014315198],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049515703,0.00020360899,0.00018327219,0.0022028564,0.00021445421,0.00059704564,0.00028707212,0.00017875606,0.0010544183],"category_scores_gemma":[0.0014082004,0.000121134035,0.00016364218,0.00089446735,0.00035401626,0.00029451426,0.00052505283,0.00012686169,0.00030398116],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003536148,0.000007078659,0.99148786,0.000009797967,0.000026382731,0.000014604373,0.00013959261,0.00025060595,0.0039077667,0.00021567907,0.00014904745,0.0037561797],"study_design_scores_gemma":[6.5478946e-7,0.0000071047343,0.9991579,0.0000016557826,0.0000030019917,0.000021227455,0.00006222867,0.00037031152,0.00020046305,0.000054958,0.000119092656,0.0000014647808],"about_ca_topic_score_codex":0.0041747973,"about_ca_topic_score_gemma":0.005746905,"teacher_disagreement_score":0.0041747973,"about_ca_system_score_codex":0.00023340563,"about_ca_system_score_gemma":0.00007945563,"threshold_uncertainty_score":0.00830102},"labels":[],"label_agreement":null},{"id":"W2617971301","doi":"10.3847/1538-4357/aab1fb","title":"Rotation and Magnetism of Massive Stellar Cores","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Angular momentum; Neutron star; Magnetic helicity; Accretion (finance); Stars; Radiative transfer; Stellar rotation; Magnetic field; Magnetohydrodynamics; Classical mechanics; Quantum mechanics","score_opus":0.008819618230543816,"score_gpt":0.22333478066384602,"score_spread":0.2145151624333022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2617971301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99831945,0.000029579292,0.00036734293,0.000013086359,0.0000021158578,0.0000016932786,0.000017826886,0.000011935715,0.0012369935],"genre_scores_gemma":[0.9997631,0.000010411997,0.00005770654,0.0000015151613,0.000001525691,6.585663e-7,0.000020533873,0.000002563428,0.00014202383],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999634,0.000007747922,0.0000019336012,0.00000843931,0.0000072094845,0.000011408546],"domain_scores_gemma":[0.99979013,0.000031783486,0.000060846316,0.00002440883,0.000026690714,0.000066031425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020080246,0.00027218938,0.00021219064,0.00040131513,0.00031982196,0.00060277455,0.00020730296,0.00020146178,0.0005996801],"category_scores_gemma":[0.00054265413,0.00014949817,0.00025114848,0.00013799264,0.00045210656,0.00025185873,0.0006270318,0.00019927372,0.00016654508],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014437225,0.00021453167,0.46849877,0.000093336705,0.000192168,0.0013184395,0.0006571405,0.27937463,0.20986532,0.022104597,0.0007930533,0.015444296],"study_design_scores_gemma":[0.00023993419,0.0010687284,0.36873612,0.000029712957,0.00008070074,0.00049770187,0.00036224868,0.58814675,0.028755086,0.0099148145,0.0021136107,0.000054532364],"about_ca_topic_score_codex":0.0029284342,"about_ca_topic_score_gemma":0.0013809568,"teacher_disagreement_score":0.0029284342,"about_ca_system_score_codex":0.00050504843,"about_ca_system_score_gemma":0.00018062757,"threshold_uncertainty_score":0.0058227777},"labels":[],"label_agreement":null},{"id":"W2618688213","doi":"10.3847/1538-4357/aa6d60","title":"Magnetically Modulated Heat Transport in a Global Simulation of Solar Magneto-convection","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Convection; Magneto; Convection zone; Magnetohydrodynamics; Astrophysics; Astronomy; Magnetic field; Computational physics; Mechanics; Thermodynamics","score_opus":0.006755227235371563,"score_gpt":0.24334955951590387,"score_spread":0.2365943322805323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2618688213","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99338114,0.00004696818,0.0014633922,0.00023674036,0.000021944246,0.000023820188,0.00031056555,0.00011147546,0.004404015],"genre_scores_gemma":[0.9984528,0.00002013786,0.00092781766,0.00003412562,0.0000067103324,0.000017613082,0.00015817948,0.000027837516,0.00035479636],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999895,0.000035892037,0.0000036158692,0.000015066036,0.000015926053,0.000034501663],"domain_scores_gemma":[0.9996166,0.00018947544,0.000032858923,0.000026956395,0.000038156188,0.00009583668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003316825,0.00044710573,0.00064091774,0.00035272853,0.00059182907,0.00081685634,0.0007192968,0.00097472384,0.001915228],"category_scores_gemma":[0.0010273336,0.00029932254,0.00054143847,0.00037693675,0.0010501082,0.00052792404,0.00084477203,0.00069571234,0.00011737958],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037445064,0.00022753332,0.010402498,0.000037304646,0.00006963287,0.000292516,0.00009942916,0.98129106,0.003842426,0.0015395228,0.00045931712,0.001364285],"study_design_scores_gemma":[0.00014972007,0.00010743744,0.0030494914,0.000004519809,0.000011935922,0.000013786198,0.000057132453,0.9952217,0.00060188625,0.00049855787,0.00027382496,0.0000100311745],"about_ca_topic_score_codex":0.012400008,"about_ca_topic_score_gemma":0.006742827,"teacher_disagreement_score":0.012400008,"about_ca_system_score_codex":0.0007621748,"about_ca_system_score_gemma":0.0006301203,"threshold_uncertainty_score":0.02465564},"labels":[],"label_agreement":null},{"id":"W2618742974","doi":"10.3847/1538-4357/aa8ccf","title":"Rise of the Titans: A Dusty, Hyper-luminous “870 μm Riser” Galaxy at z ∼ 6","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Redshift; Galaxy; Millimeter; Submillimeter Array; Infrared; Luminosity; Star formation; Luminous infrared galaxy; Astronomy","score_opus":0.009888739942636553,"score_gpt":0.21849439303097395,"score_spread":0.2086056530883374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2618742974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99876034,0.000021918391,0.00011300955,0.000018622984,0.0000019873157,0.0000026829464,0.00005326665,0.000017921508,0.0010100799],"genre_scores_gemma":[0.9993149,0.0000092022865,0.0002234233,0.00001636914,0.0000034829648,0.0000011259506,0.00012190938,0.0000023288912,0.00030728267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993014,0.000005054605,0.0000021798755,0.000017987182,0.00002408124,0.000020543594],"domain_scores_gemma":[0.99987483,0.0000069652447,0.00002897705,0.000015108941,0.000016029806,0.00005816348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010813707,0.00011771283,0.00010599488,0.00036636266,0.00043855302,0.0003233357,0.00023328794,0.00011527946,0.0010404325],"category_scores_gemma":[0.00011909533,0.00010577416,0.00011499104,0.0001326834,0.00034307508,0.00011952994,0.00031781982,0.00023108875,0.00029407602],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019598007,0.000108742905,0.8012017,0.000026236574,0.00004682852,0.0026016752,0.0011969669,0.00019060545,0.18005052,0.00076110184,0.0010671915,0.0125525],"study_design_scores_gemma":[0.0000067438446,0.00013328393,0.98768264,0.0000032689413,0.000011177736,0.0018626783,0.0002813978,0.0005959342,0.006398089,0.00008431604,0.0029364806,0.000003905365],"about_ca_topic_score_codex":0.002795497,"about_ca_topic_score_gemma":0.0046868892,"teacher_disagreement_score":0.002795497,"about_ca_system_score_codex":0.0002894891,"about_ca_system_score_gemma":0.0001439242,"threshold_uncertainty_score":0.0055584908},"labels":[],"label_agreement":null},{"id":"W2618780891","doi":"10.3847/1538-4357/aac5f8","title":"Constraints on the Mass, Concentration, and Nonthermal Pressure Support of Six CLASH Clusters from a Joint Analysis of X-Ray, SZ, and Lensing Data","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Intracluster medium; Redshift; Galaxy cluster; Weak gravitational lensing; Galaxy; Cosmology; Cluster (spacecraft)","score_opus":0.017191040631123155,"score_gpt":0.22727971936747882,"score_spread":0.21008867873635567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2618780891","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942744,0.00002364081,0.0002864643,0.0000071292693,4.104556e-7,0.0000020708137,0.00015314067,0.00001164479,0.00008818635],"genre_scores_gemma":[0.9985643,0.000015184744,0.00057500316,0.0000037478037,0.0000021917756,0.0000020628213,0.0007821769,0.00000590091,0.000049477596],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995222,0.00006849537,0.000035639427,0.00013575517,0.00014689137,0.00009105022],"domain_scores_gemma":[0.997863,0.0004960603,0.0006024096,0.00032861036,0.00021616601,0.0004938458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011178699,0.0004876421,0.0004947395,0.0025296935,0.0005284492,0.0010853258,0.0005974535,0.0002722239,0.0007170574],"category_scores_gemma":[0.0022612433,0.0004320275,0.0006314333,0.0011274135,0.00045331768,0.00034697613,0.0014974652,0.00032036638,0.00013848749],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050846767,0.0000772327,0.933326,0.000046231187,0.0003665042,0.00025973207,0.0003232905,0.016940335,0.039574344,0.0006394706,0.00027053824,0.007667814],"study_design_scores_gemma":[0.000023405515,0.000081932805,0.9495658,0.000008925632,0.000086646054,0.00011863585,0.00018471241,0.042871866,0.0063640815,0.00028331982,0.00037785972,0.000032798904],"about_ca_topic_score_codex":0.011968528,"about_ca_topic_score_gemma":0.016592626,"teacher_disagreement_score":0.011968528,"about_ca_system_score_codex":0.0006193662,"about_ca_system_score_gemma":0.0005175753,"threshold_uncertainty_score":0.02379769},"labels":[],"label_agreement":null},{"id":"W2619018213","doi":"10.3847/1538-4357/aa8456","title":"Simultaneous X-Ray, Gamma-Ray, and Radio Observations of the Repeating Fast Radio Burst FRB 121102","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Herzberg Institute of Astrophysics","funders":"","keywords":"Fast radio burst; Flux (metallurgy); Fluence; Photon; Radio frequency; Gamma-ray burst","score_opus":0.017728715540750926,"score_gpt":0.2392581771637865,"score_spread":0.22152946162303558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2619018213","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995259,0.00022255872,0.00041811625,0.000054831005,0.000015011493,0.000017195815,0.0011174745,0.00010273855,0.0027929991],"genre_scores_gemma":[0.9937463,0.00011117588,0.0011791356,0.000076202385,0.000026280572,0.00002387234,0.003860175,0.00004104092,0.00093572633],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996575,0.000023029423,0.000024357088,0.00009053538,0.00011480118,0.000089859874],"domain_scores_gemma":[0.99887675,0.00012463008,0.00040749088,0.00013744498,0.00016520129,0.00028848674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043687754,0.00061318075,0.0006096053,0.0015625561,0.0006515985,0.0008742215,0.0006349912,0.0005446886,0.002416837],"category_scores_gemma":[0.0007553721,0.0003674911,0.00036533098,0.0009753133,0.0002248533,0.00026935304,0.00068349845,0.00052717485,0.0009980648],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015011518,0.00035402022,0.5474612,0.00015965436,0.000314906,0.002196107,0.00064576516,0.0019340133,0.40055913,0.0002710076,0.002911733,0.041691337],"study_design_scores_gemma":[0.000032083102,0.0001805767,0.99189186,0.00001992235,0.000034461562,0.0006693057,0.000120666875,0.00068854535,0.0040703234,0.00004674015,0.0022231096,0.0000224401],"about_ca_topic_score_codex":0.008371906,"about_ca_topic_score_gemma":0.013185965,"teacher_disagreement_score":0.008371906,"about_ca_system_score_codex":0.0007087499,"about_ca_system_score_gemma":0.00023118287,"threshold_uncertainty_score":0.016646385},"labels":[],"label_agreement":null},{"id":"W2619972505","doi":"10.3847/1538-4357/aa80e1","title":"No Snowball on Habitable Tidally Locked Planets","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"","keywords":"Tidal locking; Planet; Astrobiology; Snowball Earth; Circumstellar habitable zone; Planetary habitability; Exoplanet; Terrestrial planet; Habitability; Physics; Geology; Environmental science; Glacial period; Astronomy; Paleontology; Spin (aerodynamics)","score_opus":0.009691565230250169,"score_gpt":0.22225618944658987,"score_spread":0.2125646242163397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2619972505","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99152136,0.00007507842,0.005444105,0.00010615498,0.000008220677,0.000008449586,0.00006332435,0.00005112156,0.002722165],"genre_scores_gemma":[0.9990477,0.000033652588,0.00038171024,0.000013992759,0.000003733764,0.0000033685872,0.000036317237,0.000011670479,0.00046793054],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999572,0.0000079768815,0.0000024487092,0.000009526722,0.0000054650263,0.000017334241],"domain_scores_gemma":[0.999749,0.000045506597,0.0000672948,0.000031925745,0.000013719194,0.000092519425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012765238,0.00019581935,0.00034301716,0.00030697006,0.00034557347,0.0008392908,0.00027509546,0.000460307,0.0021871428],"category_scores_gemma":[0.00066976174,0.00015213092,0.00073205953,0.00011143163,0.00072254194,0.0007898773,0.0008499572,0.00033735108,0.00016072197],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087411463,0.00019055356,0.16990587,0.00020139254,0.00026051508,0.003002246,0.0010684117,0.6113037,0.10835962,0.079019755,0.0015191167,0.024294768],"study_design_scores_gemma":[0.000052864903,0.00018403109,0.050733022,0.000022179393,0.000040971507,0.0002673021,0.0003247507,0.9118415,0.004114136,0.03134386,0.0010446555,0.000030743417],"about_ca_topic_score_codex":0.0036768245,"about_ca_topic_score_gemma":0.0024024486,"teacher_disagreement_score":0.0036768245,"about_ca_system_score_codex":0.0005007061,"about_ca_system_score_gemma":0.0002543411,"threshold_uncertainty_score":0.0073167086},"labels":[],"label_agreement":null},{"id":"W2621103605","doi":"10.3847/1538-4357/aa890a","title":"The Evaporation Valley in the Kepler Planets","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":738,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Photoevaporation; Planet; Exoplanet; RADIUS; Transit (satellite); Terrestrial planet; Planetary migration; Planetary system","score_opus":0.01844063171528964,"score_gpt":0.2534426247380738,"score_spread":0.23500199302278413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2621103605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9901759,0.00032250347,0.0040221615,0.00022268567,0.0000055589207,0.00000398638,0.00008841568,0.000046625977,0.005112113],"genre_scores_gemma":[0.9993026,0.000037494792,0.000221096,0.000012373481,0.0000026769944,0.0000016251571,0.000041819923,0.0000050703916,0.00037529654],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993014,0.000010627245,0.0000028710106,0.000024270668,0.000010962488,0.000021131431],"domain_scores_gemma":[0.99978584,0.00006477955,0.00005721117,0.000022296023,0.000023337216,0.000046531433],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002701611,0.00011392385,0.00025885671,0.00024550332,0.0005648852,0.0009317544,0.00027191004,0.00028068398,0.0016620696],"category_scores_gemma":[0.00090539776,0.00015228751,0.00029260496,0.00017964235,0.00047360457,0.0006271232,0.0006378119,0.000489157,0.00017532379],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093500456,0.00022697839,0.58528066,0.00025368232,0.00018574315,0.0034822423,0.002113831,0.1211971,0.068613335,0.1664909,0.0049199057,0.046300717],"study_design_scores_gemma":[0.00008649577,0.0002995788,0.5198498,0.000067646426,0.00005599685,0.0031181644,0.0016443038,0.32534602,0.014119738,0.11542335,0.01989366,0.00009537547],"about_ca_topic_score_codex":0.0019296216,"about_ca_topic_score_gemma":0.0011705573,"teacher_disagreement_score":0.0019296216,"about_ca_system_score_codex":0.0006751733,"about_ca_system_score_gemma":0.00024889628,"threshold_uncertainty_score":0.0055602193},"labels":[],"label_agreement":null},{"id":"W2622192057","doi":"10.3847/1538-4357/aa745a","title":"The Origin of B-type Runaway Stars: Non-LTE Abundances as a Diagnostic","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Queen's University; Queen's University Belfast","keywords":"Stars; Supernova; Abundance (ecology); Balmer series; Cluster (spacecraft); Line (geometry); RADIUS; Atmosphere (unit); Stellar evolution","score_opus":0.0134208801942503,"score_gpt":0.2686713905367032,"score_spread":0.2552505103424529,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2622192057","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982002,0.00031282005,0.0003248892,0.000015422804,0.000003950673,0.0000039477422,0.00011870966,0.000013825573,0.0010061907],"genre_scores_gemma":[0.9996617,0.000025321771,0.00013018523,0.000006303328,0.0000016120667,0.0000013828493,0.00008419776,0.0000024336723,0.00008690579],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973494,0.000051775416,0.000028071308,0.00006190763,0.00007340133,0.00004977507],"domain_scores_gemma":[0.9988955,0.0003123628,0.0002511685,0.00012511903,0.00019101496,0.00022477482],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037418996,0.00026353615,0.00027501915,0.0012941295,0.0003942861,0.0005416963,0.0004707288,0.00028235262,0.0016644219],"category_scores_gemma":[0.0013394655,0.000091101625,0.00014361835,0.00059017097,0.00043686753,0.00032427878,0.00062681996,0.00018624868,0.00044680643],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002994788,0.00002170889,0.98366725,0.000023725373,0.000027634034,0.0002893845,0.00015746607,0.00013436623,0.011086141,0.0001714723,0.000050864004,0.004070495],"study_design_scores_gemma":[0.0000064497303,0.00009367292,0.99386024,0.000008715199,0.000017674394,0.0006627911,0.00027882002,0.00067267497,0.0036387031,0.00026070056,0.0004953223,0.000004232415],"about_ca_topic_score_codex":0.0036451938,"about_ca_topic_score_gemma":0.003522148,"teacher_disagreement_score":0.0036451938,"about_ca_system_score_codex":0.00029855306,"about_ca_system_score_gemma":0.000112608985,"threshold_uncertainty_score":0.007247925},"labels":[],"label_agreement":null},{"id":"W2623674299","doi":"10.3847/1538-4357/aa7844","title":"The JCMT Transient Survey: Data Reduction and Calibration Methods","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Brightness; Physics; Astrophysics; Star formation; Wavelength; James Clerk Maxwell Telescope; Calibration; Data reduction; Astronomy; Remote sensing; Optics; Stars; Computer science; Geology","score_opus":0.06150983140616827,"score_gpt":0.3534256991198835,"score_spread":0.2919158677137152,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2623674299","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6593459,0.00050043676,0.22516145,0.00044241248,0.0001074015,0.00566503,0.0890258,0.008318383,0.011433185],"genre_scores_gemma":[0.45725894,0.00037410128,0.39605796,0.0002514135,0.00016968712,0.009656532,0.12887299,0.001730627,0.0056277066],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9973201,0.0004556374,0.0003742831,0.00058363564,0.001042858,0.00022348037],"domain_scores_gemma":[0.9935721,0.000541991,0.0012598116,0.0023657833,0.0020439236,0.00021640741],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002808928,0.00064499455,0.00048706465,0.005698256,0.0010602095,0.0009927143,0.0012913967,0.0006105481,0.0036226509],"category_scores_gemma":[0.006662664,0.00048100806,0.00065652456,0.008407673,0.00049419113,0.00041183358,0.0013577621,0.00066728395,0.0037593243],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061126327,0.0011439102,0.46839532,0.00050912943,0.00027490116,0.0004333607,0.0013151894,0.016571542,0.07246428,0.0026107803,0.03694007,0.39873028],"study_design_scores_gemma":[0.000071636096,0.000106361396,0.93429494,0.000032364354,0.00006982465,0.00019234577,0.00027855032,0.014756492,0.011756865,0.0004722525,0.037914146,0.000054196942],"about_ca_topic_score_codex":0.020916814,"about_ca_topic_score_gemma":0.024084898,"teacher_disagreement_score":0.020916814,"about_ca_system_score_codex":0.000974034,"about_ca_system_score_gemma":0.0016513129,"threshold_uncertainty_score":0.041590154},"labels":[],"label_agreement":null},{"id":"W2624449111","doi":"10.3847/1538-4357/aac88a","title":"Globular Clusters in a Cosmological N-body Simulation","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Halo; Astronomy; Milky Way; Redshift; Star cluster; Galactic halo; Star formation; Stars; Galaxy","score_opus":0.014642359143430728,"score_gpt":0.2575088632977791,"score_spread":0.24286650415434838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2624449111","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.983132,0.00009465097,0.0035932192,0.00038173998,0.00004927193,0.000061642386,0.0012893042,0.0003099088,0.011088353],"genre_scores_gemma":[0.9914743,0.000062536856,0.005077858,0.00012983233,0.000016579279,0.000068599635,0.0010990826,0.00007064862,0.0020006278],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985695,0.000054263528,0.0000047604194,0.000029944025,0.000023988048,0.000030077254],"domain_scores_gemma":[0.9990527,0.00047882408,0.00006376708,0.000064273656,0.000116683055,0.00022376978],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006119492,0.0004536618,0.00057702436,0.00047666577,0.0006821228,0.00088074553,0.0015915441,0.0012090742,0.0044040564],"category_scores_gemma":[0.0024072486,0.00034861706,0.0006177842,0.00064361445,0.00068851945,0.0004736168,0.00093878666,0.0009870342,0.00041602226],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002852618,0.00019326313,0.012867061,0.000038143226,0.00008804653,0.00018470919,0.00010066619,0.97852314,0.00059264957,0.0044779675,0.0011311303,0.0015178767],"study_design_scores_gemma":[0.00014705898,0.0000630669,0.0023223332,0.0000058817977,0.000019290548,0.000012730772,0.0000512631,0.9958086,0.00014579133,0.0008290209,0.00058471423,0.0000102452],"about_ca_topic_score_codex":0.058873467,"about_ca_topic_score_gemma":0.035035696,"teacher_disagreement_score":0.058873467,"about_ca_system_score_codex":0.0012782589,"about_ca_system_score_gemma":0.0011481625,"threshold_uncertainty_score":0.117061615},"labels":[],"label_agreement":null},{"id":"W2625743954","doi":"10.3847/1538-4357/aa77f6","title":"Magnetohydrodynamic Models of Molecular Tornadoes","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Molecular cloud; Dimensionless quantity; Equipartition theorem; Toroid; Classical mechanics; Mechanics; Astrophysics; Magnetic field; Plasma; Stars; Quantum mechanics","score_opus":0.009360403118400215,"score_gpt":0.23703564347510592,"score_spread":0.2276752403567057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2625743954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94091886,0.00027538466,0.043422394,0.00052154943,0.00003325661,0.000036313617,0.00016222119,0.0001338392,0.014496206],"genre_scores_gemma":[0.9980627,0.000053299333,0.0009666641,0.000012951849,0.000011657048,0.000015542664,0.000029569117,0.000008420763,0.0008393095],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999454,0.000015427964,0.000002060928,0.000010363882,0.000009369811,0.000017407325],"domain_scores_gemma":[0.9998673,0.000025651934,0.000047855065,0.000010662156,0.000014015969,0.000034496534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013489973,0.00029210714,0.00029406033,0.0003457148,0.00046439894,0.00076174276,0.0007983266,0.0005272243,0.0013495474],"category_scores_gemma":[0.00048925,0.00017914597,0.00034860792,0.00019599979,0.0008745377,0.00053587556,0.00045649623,0.0002500761,0.00012429633],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057178204,0.000035603352,0.0046297414,0.000019311608,0.00003178373,0.00046827292,0.00017489589,0.89902246,0.0034594596,0.08999716,0.0005741267,0.0015299792],"study_design_scores_gemma":[0.000021003836,0.000012389286,0.0015829556,0.0000028288412,0.00000317132,0.00004291428,0.000046550103,0.98536533,0.0001317521,0.012300607,0.00048352848,0.000006985476],"about_ca_topic_score_codex":0.009346141,"about_ca_topic_score_gemma":0.002872647,"teacher_disagreement_score":0.009346141,"about_ca_system_score_codex":0.00080745586,"about_ca_system_score_gemma":0.00025002795,"threshold_uncertainty_score":0.018583477},"labels":[],"label_agreement":null},{"id":"W2625884697","doi":"10.3847/1538-4357/aa9a40","title":"HST Imaging of the Brightest z ∼ 8–9 Galaxies from UltraVISTA: The Extreme Bright End of the UV Luminosity Function","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Japan Society for the Promotion of Science; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; High Energy Accelerator Research Organization; Los Alamos National Laboratory; National Astronomical Observatory of Japan; National Central University; Centre National de la Recherche Scientifique; Eötvös Loránd Tudományegyetem; Academia Sinica; Space Telescope Science Institute; Ministry of Education, Culture, Sports, Science and Technology; Princeton University; Johns Hopkins University; National Aeronautics and Space Administration; Japan Science and Technology Agency; Cabinet Office, Government of Japan; Durham University; Smithsonian Institution; Toray Science Foundation; National Science Foundation","keywords":"Galaxy; Luminosity function; Luminosity; Luminous infrared galaxy; Active galactic nucleus; Spectral energy distribution; Photometry (optics)","score_opus":0.009836418070871576,"score_gpt":0.19966277243817612,"score_spread":0.18982635436730455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2625884697","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979911,0.000054708653,0.00033957342,0.000019695564,0.0000019224947,0.0000038413336,0.0002677722,0.000058603207,0.0012628065],"genre_scores_gemma":[0.99798054,0.00002913493,0.0007705545,0.000028145758,0.000005128975,0.0000035105695,0.0008206364,0.000011503208,0.00035082854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990857,0.000006213941,0.0000037489249,0.000021655573,0.00003234987,0.00002751267],"domain_scores_gemma":[0.9996637,0.000019464136,0.00011289924,0.00004572526,0.000047819594,0.00011051745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016419547,0.00013750036,0.00018356268,0.0009943703,0.0004403111,0.0006821602,0.00030158233,0.00020782303,0.0011612346],"category_scores_gemma":[0.00016501965,0.00018007727,0.0002731169,0.00044018266,0.00021133614,0.0001927379,0.0005415985,0.00027572748,0.00040725872],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021194684,0.00010346876,0.8947955,0.000018923018,0.00006213738,0.0003184246,0.00041997328,0.00023330524,0.0889966,0.00023044381,0.0006359324,0.013973347],"study_design_scores_gemma":[0.0000059079466,0.00003620344,0.9960217,0.000004256723,0.000009855188,0.00017739112,0.00009080111,0.00032033827,0.0026727247,0.000039624327,0.0006176558,0.0000035464266],"about_ca_topic_score_codex":0.0066102496,"about_ca_topic_score_gemma":0.016216012,"teacher_disagreement_score":0.0066102496,"about_ca_system_score_codex":0.00030844685,"about_ca_system_score_gemma":0.00015640772,"threshold_uncertainty_score":0.013143539},"labels":[],"label_agreement":null},{"id":"W2626140264","doi":"10.3847/1538-4357/aa738d","title":"Variable Stars in Local Group Galaxies. III. And VII, NGC 147, and NGC 185: Insight into the Building Blocks of the M31 Halo<sup>∗</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"RR Lyrae variable; Physics; Astrophysics; Variable star; Astronomy; Spiral galaxy; Galaxy; Globular cluster; Stars; Local Group; Cepheid variable; Milky Way; Halo; Galactic halo; Dwarf spheroidal galaxy; Dwarf galaxy; Population; Interacting galaxy","score_opus":0.0072019897364322865,"score_gpt":0.21174697431261208,"score_spread":0.20454498457617978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2626140264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986821,0.00027185355,0.000061356615,0.00001980237,5.906276e-7,0.0000019239928,0.00015642907,0.0000066161133,0.0007993658],"genre_scores_gemma":[0.99931407,0.00009390102,0.00014375744,0.000008357112,0.0000023310247,0.0000015548911,0.00027120914,0.000002527161,0.00016230988],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999528,0.0000058177247,0.0000034695984,0.000013745685,0.0000109655175,0.000013242956],"domain_scores_gemma":[0.9996594,0.000076229415,0.0001281589,0.000032776294,0.000031609943,0.00007191148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001774806,0.00009217892,0.00014117504,0.0012859942,0.00020076148,0.0004331504,0.00014568798,0.00017823238,0.0018618859],"category_scores_gemma":[0.00035689818,0.00007816483,0.00014752444,0.0008367598,0.0003305757,0.00023988645,0.00034002538,0.0000826418,0.00033284948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000074628275,0.000010182324,0.9844238,0.000031314932,0.000016657585,0.00016385458,0.00049617735,0.00016621538,0.006646787,0.00021738342,0.00016504682,0.007588082],"study_design_scores_gemma":[0.0000015198576,0.000017267084,0.9983846,0.000005127285,0.000009199174,0.00018079077,0.0002965886,0.0001204502,0.00046692256,0.00010073612,0.00041474198,0.0000020379978],"about_ca_topic_score_codex":0.004237044,"about_ca_topic_score_gemma":0.008710968,"teacher_disagreement_score":0.004237044,"about_ca_system_score_codex":0.00030727166,"about_ca_system_score_gemma":0.00011471428,"threshold_uncertainty_score":0.008424759},"labels":[],"label_agreement":null},{"id":"W2626250038","doi":"10.3847/1538-4357/aa86f0","title":"Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-based Cross-correlation Search in Advanced LIGO Data","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Royal Society; Ministerio de Economía y Competitividad; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Govern de les Illes Balears; European Commission; Abdus Salam International Centre for Theoretical Physics; National Research Foundation; Russian Foundation for Basic Research; Scottish Universities Physics Alliance; Leverhulme Trust; Scottish Funding Council; Istituto Nazionale di Fisica Nucleare; Kavli Foundation; Science and Engineering Research Board; National Science Foundation; Hungarian Scientific Research Fund","keywords":"Physics; LIGO; Gravitational wave; Astrophysics; Astronomy; Gravitational-wave observatory","score_opus":0.04370117846550788,"score_gpt":0.38375369989205316,"score_spread":0.3400525214265453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2626250038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99499583,0.000111911875,0.0037442197,0.000088180146,0.0000019270547,0.0000050562,0.00012460003,0.00007308014,0.00085524446],"genre_scores_gemma":[0.99813265,0.000019823758,0.0013846084,0.000015731417,0.0000040324367,0.0000037537154,0.00035194287,0.0000102727945,0.000077206154],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99918467,0.00029820183,0.00003257269,0.0001757065,0.00021096547,0.000097943805],"domain_scores_gemma":[0.99627906,0.0022952121,0.0005707516,0.0004291467,0.00021289996,0.00021286038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003569956,0.0004567269,0.00044401304,0.0012895531,0.00040383905,0.0010600681,0.0005656681,0.00055630173,0.0009923257],"category_scores_gemma":[0.0062049283,0.00025461722,0.000516446,0.0005159734,0.0006785021,0.0006400458,0.0011304865,0.00042636777,0.00011882354],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015953343,0.0003145988,0.53119576,0.00020209231,0.0004930496,0.00055467524,0.00041567654,0.3910692,0.036652293,0.007920795,0.0014730606,0.028113587],"study_design_scores_gemma":[0.0001986934,0.00036689395,0.32364783,0.00006178724,0.00015199538,0.00028687765,0.00013127772,0.65345794,0.015009784,0.0055084135,0.001103031,0.000075443415],"about_ca_topic_score_codex":0.0030334927,"about_ca_topic_score_gemma":0.0029056547,"teacher_disagreement_score":0.003569956,"about_ca_system_score_codex":0.0007726593,"about_ca_system_score_gemma":0.00046751497,"threshold_uncertainty_score":0.01888001},"labels":[],"label_agreement":null},{"id":"W2626682469","doi":"10.3847/1538-4357/aa77b1","title":"The Next Generation Virgo Cluster Survey (NGVS). XXVI. The Issues of Photometric Age and Metallicity Estimates for Globular Clusters","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Physics; Metallicity; Virgo Cluster; Astronomy; Astrophysics; Cluster (spacecraft); Galaxy cluster; Stars; Galaxy","score_opus":0.052845864346094014,"score_gpt":0.2942431054098368,"score_spread":0.24139724106374277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2626682469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9347615,0.0025775114,0.0062901885,0.00072311814,0.00012925641,0.00006658659,0.045282554,0.000422294,0.009747012],"genre_scores_gemma":[0.9547693,0.00051127904,0.0048495755,0.00012697802,0.000029463743,0.000042218908,0.03619091,0.000083239356,0.003396984],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971503,0.00007790169,0.000013831561,0.0000649177,0.00008109739,0.000047248097],"domain_scores_gemma":[0.9994578,0.00011110534,0.00010522081,0.0001425908,0.000116754076,0.0000665423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008847037,0.00022992503,0.00022561653,0.0012062886,0.00024976325,0.0006225749,0.00054018816,0.00020349331,0.0018170167],"category_scores_gemma":[0.0016005688,0.00010584065,0.0003498883,0.0009663542,0.00015826226,0.0003549874,0.0004934989,0.00015965887,0.000681884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014348212,0.000027244756,0.928615,0.000108517,0.00013494962,0.0000789125,0.00013464253,0.0082190065,0.0019544503,0.0028776997,0.01555115,0.042154953],"study_design_scores_gemma":[0.000009420105,0.00002678218,0.9689792,0.00003566531,0.000031715,0.000063260464,0.00014084356,0.010770172,0.0010523134,0.0015242267,0.017356303,0.000010219003],"about_ca_topic_score_codex":0.047729023,"about_ca_topic_score_gemma":0.058192506,"teacher_disagreement_score":0.047729023,"about_ca_system_score_codex":0.0011529768,"about_ca_system_score_gemma":0.0005031521,"threshold_uncertainty_score":0.094902396},"labels":[],"label_agreement":null},{"id":"W2634689578","doi":"10.3847/1538-4357/aa92c9","title":"Constraints on the Distance Moduli, Helium, and Metal Abundances, and Ages of Globular Clusters from Their RR Lyrae and Non-variable Horizontal Branch Stars. II. Multiple Stellar Populations in 47 Tuc, M3, and M13","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Globular cluster; Horizontal branch; RR Lyrae variable; Stellar evolution; Red-giant branch; Star cluster; Stellar population; Stars; Population","score_opus":0.01563716723060866,"score_gpt":0.22723188227795374,"score_spread":0.2115947150473451,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2634689578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998609,0.00003004487,0.0006573969,0.00002771154,0.0000018393115,0.0000026830874,0.00018827987,0.00002379226,0.00045929698],"genre_scores_gemma":[0.9989177,0.000016201997,0.00056679087,0.000009254485,0.000001854795,0.0000051473908,0.00036518188,0.000019827074,0.000097954995],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999027,0.000021195116,0.0000049707355,0.00002003027,0.000018768682,0.000032303993],"domain_scores_gemma":[0.99933416,0.00031083965,0.0000758942,0.00007191647,0.00008613992,0.00012104448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004971431,0.0004181773,0.00031359794,0.0003668479,0.00048856076,0.0005762994,0.0006336491,0.00065690605,0.0013358563],"category_scores_gemma":[0.0016742336,0.0002884681,0.0005601203,0.0003968976,0.00030640693,0.00036614074,0.00041727698,0.00035370913,0.000303991],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040434088,0.00009276914,0.26524526,0.000049824946,0.0001101393,0.0002204996,0.00020148896,0.7135381,0.010738758,0.0021493796,0.0008668044,0.00638262],"study_design_scores_gemma":[0.00008828761,0.000060608334,0.09750325,0.000016844699,0.000035412053,0.00005882473,0.00015375637,0.8961845,0.004073396,0.0012382786,0.0005654353,0.000021282325],"about_ca_topic_score_codex":0.017189568,"about_ca_topic_score_gemma":0.016745692,"teacher_disagreement_score":0.017189568,"about_ca_system_score_codex":0.0014355527,"about_ca_system_score_gemma":0.0006353111,"threshold_uncertainty_score":0.03417903},"labels":[],"label_agreement":null},{"id":"W2639412928","doi":"10.3847/1538-4357/aa7755","title":"The Next Generation Virgo Cluster Survey. XXVIII. Characterization of the Galactic White Dwarf Population","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria; Queen's University","funders":"Canadian Space Agency; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; Deutsche Forschungsgemeinschaft; New Mexico State University; University of Portsmouth; Universität Basel; Canadian Foundation for AIDS Research; U.S. Department of Energy; U.S. Naval Observatory; Canarie; University of Pittsburgh; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; Princeton University; Johns Hopkins University; Ohio State University; Fermilab; Case Western Reserve University; National Science Foundation; Natural Sciences and Engineering Research Council of Canada; Drexel University; National Aeronautics and Space Administration","keywords":"Halo; White dwarf; Sky; Galactic halo; Photometry (optics); Virgo Cluster; Proper motion; Population; Globular cluster","score_opus":0.03134200582190807,"score_gpt":0.24688629688428299,"score_spread":0.2155442910623749,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2639412928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9772092,0.00032821504,0.00060709624,0.00007271647,0.0000073624274,0.000040565712,0.015990136,0.000058472975,0.0056862435],"genre_scores_gemma":[0.9667554,0.00017124228,0.0013087498,0.000039378512,0.000007708501,0.000042911284,0.029423388,0.000017025215,0.0022341562],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998964,0.000015307429,0.000005813692,0.000025057505,0.000037319944,0.000020014217],"domain_scores_gemma":[0.99979514,0.00001941258,0.000058161117,0.000026666881,0.00004314622,0.00005751582],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025320344,0.00014823371,0.00011470761,0.001608477,0.00018215633,0.00024939535,0.00017697601,0.000112845795,0.0014103854],"category_scores_gemma":[0.00046879234,0.000058206835,0.00017409654,0.00063478516,0.000087376175,0.00014759126,0.00034586416,0.000103649916,0.00060104975],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054128155,0.000013114262,0.9870712,0.00002202327,0.000026554346,0.00003914606,0.00009889819,0.0007866232,0.0016897395,0.0003639561,0.0025439835,0.007290613],"study_design_scores_gemma":[0.0000022289917,0.0000076808055,0.9971228,0.0000033875842,0.0000034802765,0.000031940788,0.0000319845,0.000856295,0.00030585512,0.00005138267,0.0015813285,0.000001700354],"about_ca_topic_score_codex":0.033243246,"about_ca_topic_score_gemma":0.04593436,"teacher_disagreement_score":0.033243246,"about_ca_system_score_codex":0.0004512278,"about_ca_system_score_gemma":0.00022082543,"threshold_uncertainty_score":0.066099465},"labels":[],"label_agreement":null},{"id":"W2645019312","doi":"10.3847/0004-637x/818/2/111","title":"PROGENITORS OF TYPE IIb SUPERNOVAE IN THE LIGHT OF RADIO AND X-RAYS FROM SN 2013df","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Analytical Chemistry (journal); Materials science; Chemistry","score_opus":0.009897184230265981,"score_gpt":0.21887893430622843,"score_spread":0.20898175007596245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2645019312","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992194,0.00006345957,0.00014636046,0.0000060065836,0.0000025658483,0.0000032513656,0.00020737028,0.000008727117,0.00034265633],"genre_scores_gemma":[0.99849117,0.000039338192,0.00020926405,0.0000075418766,0.0000044178882,0.000005584543,0.0010592003,0.0000060842267,0.00017732388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999224,0.000007045675,0.0000069838406,0.000018531942,0.000018753397,0.000026232763],"domain_scores_gemma":[0.99965894,0.000027097987,0.000114311464,0.000022935232,0.00004234489,0.00013441902],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026326114,0.0004240978,0.0005252861,0.0009147069,0.00045791944,0.00074662105,0.0002853476,0.00026704912,0.0008978004],"category_scores_gemma":[0.0004760846,0.0002013675,0.00043687274,0.00055380934,0.00018870909,0.00014777617,0.0006761814,0.00035547488,0.00032070067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002968932,0.000051500378,0.972844,0.000020575228,0.000062884996,0.0006210479,0.00016711971,0.00070673134,0.020804686,0.00017470839,0.00014886106,0.0041009886],"study_design_scores_gemma":[0.0000039760926,0.00005594671,0.9973544,0.000005473758,0.000016594851,0.0003547391,0.00009012887,0.00077395624,0.00083639467,0.00008491828,0.0004182372,0.0000052690943],"about_ca_topic_score_codex":0.0068202554,"about_ca_topic_score_gemma":0.0077735637,"teacher_disagreement_score":0.0068202554,"about_ca_system_score_codex":0.00041256464,"about_ca_system_score_gemma":0.00021169594,"threshold_uncertainty_score":0.01356113},"labels":[],"label_agreement":null},{"id":"W2676356478","doi":"10.3847/0004-637x/827/1/62","title":"STATE-SPECIFIC DISSOCIATION RATES FOR H<sub>2</sub>(v, j) + H<sub>2</sub>(v′, j′)","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Northern British Columbia","funders":"","keywords":"Physics; Dissociation (chemistry); Atomic physics; Excitation; Bond-dissociation energy; Internal energy; Energy (signal processing); Piecewise; Thermodynamics; Molecule; Physical chemistry; Quantum mechanics; Chemistry; Mathematical analysis","score_opus":0.0100739347957251,"score_gpt":0.2529770038703704,"score_spread":0.24290306907464532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2676356478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9828199,0.00010370819,0.0139086675,0.000043287084,0.000011307326,0.000025807156,0.00054783863,0.00009336011,0.0024460037],"genre_scores_gemma":[0.9945732,0.00007730806,0.0029875173,0.000008165626,0.0000014293701,0.000031132557,0.0006177697,0.00004900979,0.0016545001],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99989533,0.000012521291,0.000005755563,0.000026918846,0.0000275632,0.00003189922],"domain_scores_gemma":[0.99954647,0.00021076691,0.00006714868,0.00005076122,0.00009375158,0.00003095883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005939832,0.00030132424,0.00024111023,0.0004202664,0.00040963403,0.00041226015,0.0005565016,0.00023497871,0.0040503964],"category_scores_gemma":[0.001273671,0.00030147453,0.00038658452,0.00038385383,0.00033447848,0.0006021119,0.00029453982,0.00043123215,0.00032342476],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011921341,0.00023208883,0.053388365,0.00040885186,0.00027740863,0.00035433323,0.0008774048,0.63007873,0.24609317,0.04183434,0.0019554,0.023307776],"study_design_scores_gemma":[0.000053316235,0.00017026362,0.02909546,0.000026907213,0.000048418067,0.00020393515,0.0002645359,0.784193,0.17857873,0.005029903,0.0022027718,0.00013282863],"about_ca_topic_score_codex":0.003902209,"about_ca_topic_score_gemma":0.0037195254,"teacher_disagreement_score":0.0040503964,"about_ca_system_score_codex":0.0011617014,"about_ca_system_score_gemma":0.00046732379,"threshold_uncertainty_score":0.013549924},"labels":[],"label_agreement":null},{"id":"W2684263115","doi":"10.3847/1538-4357/aa767b","title":"Measuring the Properties of Dark Energy with Photometrically Classified Pan-STARRS Supernovae. I. Systematic Uncertainty from Core-collapse Supernova Contamination","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; FAS Division of Science, Harvard University; Australian Astronomical Optics-Macquarie; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Centre National de la Recherche Scientifique; Ministério da Ciência, Tecnologia e Inovação; Centre National d’Etudes Spatiales; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Institut national des sciences de l'Univers; Vanderbilt University; University of Chicago; Harvard University; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Yale University; National Science Foundation","keywords":"Supernova; Galaxy; Dark energy; Redshift; Prior probability; Abundance (ecology); Spectral line; Lambda","score_opus":0.0345571781399441,"score_gpt":0.2252647718614415,"score_spread":0.1907075937214974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2684263115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98482174,0.00015511336,0.013853585,0.000027472272,0.0000056942195,0.000014879759,0.00034633267,0.00014718984,0.0006279791],"genre_scores_gemma":[0.99561995,0.00002816726,0.0037996552,0.000010279507,0.0000040105915,0.000007231654,0.00045948915,0.000019469942,0.00005174348],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9983475,0.00066639594,0.00012035937,0.00041607348,0.00038597712,0.000063753985],"domain_scores_gemma":[0.98647565,0.005979426,0.0031812387,0.0029006724,0.0011378778,0.00032521217],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0054864693,0.000577636,0.00039158217,0.0012615853,0.0003710084,0.00074086594,0.00087068556,0.0004045268,0.00038608606],"category_scores_gemma":[0.016317856,0.0005231834,0.0007171438,0.0010779969,0.000607062,0.00076364586,0.00086100283,0.0003804151,0.000108989065],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021673199,0.000058109752,0.921866,0.000040236555,0.00048250012,0.000031371306,0.000080526814,0.058298174,0.0065850248,0.0010408787,0.00012572647,0.011174659],"study_design_scores_gemma":[0.000036798872,0.00019683094,0.6779733,0.000035984773,0.00014500841,0.00014654097,0.000066796776,0.2982139,0.020061,0.0023640152,0.00069000485,0.00006988435],"about_ca_topic_score_codex":0.006291875,"about_ca_topic_score_gemma":0.009150892,"teacher_disagreement_score":0.006291875,"about_ca_system_score_codex":0.00095709687,"about_ca_system_score_gemma":0.0002842628,"threshold_uncertainty_score":0.0290156},"labels":[],"label_agreement":null},{"id":"W269439282","doi":"10.1088/0004-637x/701/1/42","title":"SUNYAEV-ZEL'DOVICH EFFECT OBSERVATIONS OF THE BULLET CLUSTER (1E 0657–56) WITH APEX-SZ","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Superconducting and THz Device Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Sunyaev–Zel'dovich effect; RADIUS; Cluster (spacecraft); Galaxy cluster; Hydrostatic equilibrium; Galaxy; Astronomy","score_opus":0.010262087442319271,"score_gpt":0.22673602639480583,"score_spread":0.21647393895248657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W269439282","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99885595,0.000047598212,0.00012305344,0.000010364247,0.000002963296,0.0000037363989,0.00014558817,0.00001708347,0.0007935783],"genre_scores_gemma":[0.9988662,0.000047274116,0.0004552757,0.00000737362,0.0000068441373,0.0000034222792,0.00035713773,0.000006090037,0.00025038433],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986506,0.0000074033483,0.000007728401,0.00003841259,0.000044836375,0.0000364882],"domain_scores_gemma":[0.99971265,0.000022578757,0.00010254012,0.000036940746,0.000026938784,0.000098366625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016760608,0.00020150232,0.0003592676,0.00040502765,0.0002494158,0.00038893978,0.00032551435,0.00017380164,0.00073058624],"category_scores_gemma":[0.00040841242,0.00017817816,0.00017083157,0.00028280928,0.00028738845,0.00015304596,0.00087487063,0.0002359947,0.0002826532],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005197177,0.00006667687,0.9363422,0.000060108014,0.00006947793,0.0004609516,0.00042120225,0.0033076627,0.044261273,0.00071826176,0.00083245203,0.012940072],"study_design_scores_gemma":[0.000025786601,0.00006295839,0.9943599,0.000007622141,0.00001737582,0.00017233408,0.00006649832,0.0016858224,0.0024445192,0.00007055762,0.0010787719,0.000007715048],"about_ca_topic_score_codex":0.005105701,"about_ca_topic_score_gemma":0.011606521,"teacher_disagreement_score":0.005105701,"about_ca_system_score_codex":0.00038400918,"about_ca_system_score_gemma":0.00016424684,"threshold_uncertainty_score":0.010151982},"labels":[],"label_agreement":null},{"id":"W2712806622","doi":"10.3847/1538-4357/aa7aa5","title":"Pixel Color–Magnitude Diagram Analysis of the Brightest Cluster Galaxies in Dynamically Young and Old Clusters Abell 1139 and Abell 2589","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Pixel; Galaxy; Surface brightness; Cluster (spacecraft); Diagram; Galaxy cluster; Virgo Cluster; Brightness","score_opus":0.004847466127936038,"score_gpt":0.21077555999990286,"score_spread":0.2059280938719668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2712806622","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99893767,0.000028491444,0.00025029623,0.0000058858864,9.539893e-7,0.0000015776037,0.0002431875,0.000023272054,0.0005087645],"genre_scores_gemma":[0.99904484,0.000007871993,0.00044208887,0.0000026331563,0.0000017369578,0.0000012811445,0.00039749392,0.000005091234,0.00009682999],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999453,0.00000531557,0.0000035659698,0.000017643582,0.000012928365,0.000015322039],"domain_scores_gemma":[0.99961036,0.00006581474,0.00010054366,0.000027445718,0.00007126172,0.00012459669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011028973,0.000079963924,0.00011970617,0.0018165576,0.00020443574,0.0003805366,0.00013206477,0.00015129925,0.0010919201],"category_scores_gemma":[0.00031337645,0.000070861846,0.00015139808,0.00075873546,0.00017278378,0.00014972457,0.00022778557,0.0001097663,0.00016974466],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002819125,0.00004582121,0.92787397,0.000025786527,0.000038631388,0.00028340644,0.0003831519,0.0013150665,0.055975486,0.00055313774,0.00037895716,0.012844695],"study_design_scores_gemma":[0.0000010500066,0.000008386865,0.9982145,6.7663956e-7,0.0000035291926,0.000048720114,0.00005520923,0.0007647756,0.0007128251,0.000030407198,0.00015814549,0.0000017306548],"about_ca_topic_score_codex":0.006772811,"about_ca_topic_score_gemma":0.0077686547,"teacher_disagreement_score":0.006772811,"about_ca_system_score_codex":0.0003130292,"about_ca_system_score_gemma":0.00009035283,"threshold_uncertainty_score":0.013466775},"labels":[],"label_agreement":null},{"id":"W2722535400","doi":"10.3847/1538-4357/aa7514","title":"Feeling the Pull: A Study of Natural Galactic Accelerometers. II. Kinematics and Mass of the Delicate Stellar Stream of the Palomar 5 Globular Cluster<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"","keywords":"Stars; Globular cluster; Physics; Astrophysics; Sky; RR Lyrae variable; Population; Star cluster","score_opus":0.01561751033401551,"score_gpt":0.24047582795443054,"score_spread":0.22485831762041503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2722535400","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989906,0.000018537785,0.00019282174,0.000012742752,0.0000016234819,0.0000058683804,0.00005487187,0.000004254352,0.0007185587],"genre_scores_gemma":[0.99885845,0.000026474732,0.00035441335,0.00001052305,0.0000019737333,0.0000055972837,0.00020004531,0.0000044829503,0.00053813745],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998946,0.000035783818,0.000005955694,0.00002571198,0.000024386623,0.000013448603],"domain_scores_gemma":[0.9993436,0.00023323545,0.00016407549,0.00006246662,0.0001097476,0.00008696218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020243341,0.0001519868,0.0001273652,0.000327085,0.00026008722,0.00040745462,0.00022383448,0.00018432458,0.0014573121],"category_scores_gemma":[0.0020177355,0.000121230405,0.00011276092,0.00024867614,0.00035544555,0.00023454448,0.00030179805,0.00016842809,0.0003490948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000348929,0.00017344647,0.96871376,0.00003141571,0.000035137553,0.00025393043,0.0016044681,0.00047233285,0.00964037,0.0005965121,0.00040228278,0.017727328],"study_design_scores_gemma":[0.000008634229,0.00027024795,0.9926966,0.0000052574965,0.000010828974,0.00016031906,0.0021679732,0.003000631,0.0008093429,0.00014176607,0.00072184013,0.000006540203],"about_ca_topic_score_codex":0.0032253927,"about_ca_topic_score_gemma":0.0069702715,"teacher_disagreement_score":0.0032253927,"about_ca_system_score_codex":0.00022321197,"about_ca_system_score_gemma":0.00012332635,"threshold_uncertainty_score":0.0064132214},"labels":[],"label_agreement":null},{"id":"W2726786188","doi":"10.3847/1538-4357/aa947b","title":"A Comparison of Cosmological Parameters Determined from CMB Temperature Power Spectra from the South Pole Telescope and the Planck Satellite","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Planck; Cosmic microwave background; Physics; South Pole Telescope; Multipole expansion; Astrophysics; Cosmic variance; Spectral density; Cold dark matter; Cosmic background radiation; Horizon; Cosmology; Astronomy; Statistics; Quantum mechanics","score_opus":0.014210275003784105,"score_gpt":0.26981812150078094,"score_spread":0.25560784649699686,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2726786188","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970784,0.000046391,0.00077344704,0.000025906957,0.0000031682757,0.0000025354643,0.0007020355,0.000019688872,0.0013484153],"genre_scores_gemma":[0.9985482,0.000016971066,0.00060019677,0.000005645825,0.000004244952,0.0000020016407,0.0007365497,0.000009098697,0.0000770518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99957126,0.000108012115,0.000022864388,0.00013227726,0.00013084868,0.000034733537],"domain_scores_gemma":[0.9976253,0.0009442587,0.00055669073,0.00041349445,0.0003142625,0.000146013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009191958,0.00021846128,0.00015329393,0.001395614,0.00017800395,0.00055138185,0.00030531487,0.00026665526,0.0015555507],"category_scores_gemma":[0.004836341,0.00020755018,0.00031658297,0.0015419562,0.00024914937,0.00056358747,0.00063684303,0.00025788468,0.00046650934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017184552,0.000015643109,0.9806818,0.000027623775,0.0002571542,0.00007200772,0.00024232229,0.0020612897,0.008111901,0.00041544696,0.00042394284,0.0075189895],"study_design_scores_gemma":[0.0000029027276,0.000012534326,0.9963742,0.0000028582344,0.000021667245,0.000027109149,0.000078772326,0.0022056166,0.0009321603,0.000077752506,0.00025948888,0.000004889198],"about_ca_topic_score_codex":0.0043905918,"about_ca_topic_score_gemma":0.005196642,"teacher_disagreement_score":0.0043905918,"about_ca_system_score_codex":0.00023105637,"about_ca_system_score_gemma":0.00012632355,"threshold_uncertainty_score":0.008730054},"labels":[],"label_agreement":null},{"id":"W2726861356","doi":"10.3847/1538-4357/aa7de0","title":"Chromospheric Inversions of a Micro-flaring Region","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Irish Centre for High-End Computing; Stockholms Universitet; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Queen's University; Science Foundation Ireland; Queen's University Belfast","keywords":"Chromosphere; Solar telescope; Sunspot; Photosphere; Astrophysics; Physics; Atmosphere (unit); Solar flare; Line (geometry); Telescope; Astronomy; Spectral line; Magnetic field; Meteorology; Geometry","score_opus":0.011566886793531298,"score_gpt":0.23119219534125682,"score_spread":0.21962530854772552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2726861356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99793005,0.00002950114,0.00077692326,0.000014551308,0.0000023758028,0.000002811993,0.00026080204,0.000074966,0.00090809923],"genre_scores_gemma":[0.9987662,0.000012191306,0.0006171572,0.0000036063698,0.000001974146,0.0000011760003,0.000418284,0.000008684139,0.00017073311],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997425,0.0000017296499,9.1839723e-7,0.00000846371,0.000005785449,0.000008714051],"domain_scores_gemma":[0.9999243,0.000012194831,0.000018775228,0.000011780945,0.000017805585,0.000015129025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000053833424,0.00011177113,0.00010581654,0.00034063126,0.00015364838,0.00023428656,0.00012593735,0.00011768511,0.0010820183],"category_scores_gemma":[0.00024132755,0.00008503106,0.00016028868,0.00033044902,0.00009600532,0.0001457173,0.00015152128,0.00018332497,0.00013592535],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009908365,0.00019498265,0.3929223,0.00008468364,0.00031453918,0.0010895263,0.00093048613,0.043270025,0.47355452,0.00079040835,0.0017214856,0.08413616],"study_design_scores_gemma":[0.000015110436,0.00004443055,0.9483185,0.0000054559246,0.00003179056,0.000158869,0.00018726969,0.040038288,0.009670563,0.00022448416,0.0012888232,0.000016377277],"about_ca_topic_score_codex":0.007746464,"about_ca_topic_score_gemma":0.015624987,"teacher_disagreement_score":0.007746464,"about_ca_system_score_codex":0.00015731457,"about_ca_system_score_gemma":0.00009933282,"threshold_uncertainty_score":0.015402734},"labels":[],"label_agreement":null},{"id":"W2727952977","doi":"10.3847/1538-4357/aa911b","title":"SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES): Faint-end Counts at 450 μm","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Saint Mary's University; Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Source counts; Redshift; Galaxy; Luminosity; Flux (metallurgy); Photometric redshift; Surface brightness; Population; Point source; Astronomy; Luminous infrared galaxy; Optics","score_opus":0.017526753939224843,"score_gpt":0.2590042702121867,"score_spread":0.24147751627296185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2727952977","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8695859,0.00042786365,0.016955925,0.00038804716,0.00005788857,0.00025561958,0.08017706,0.0021813952,0.029970368],"genre_scores_gemma":[0.8780673,0.00014136184,0.024309484,0.00029711853,0.00015858354,0.00026087053,0.089599065,0.00048324745,0.006683003],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995832,0.00007366148,0.00002376143,0.000097254204,0.00013477208,0.000087422806],"domain_scores_gemma":[0.99861693,0.00016217964,0.00029421263,0.0003612946,0.0002878932,0.00027752187],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008214242,0.00035218368,0.00027045983,0.0023445217,0.00036121812,0.0007267573,0.0006440572,0.00025204394,0.0042527285],"category_scores_gemma":[0.0012460747,0.0002503729,0.0004309959,0.0017892452,0.0001616176,0.00036945767,0.0007517901,0.00035787906,0.0013940558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000542505,0.0001417854,0.8447224,0.0001354347,0.00020721399,0.00023823474,0.00042097495,0.0038901032,0.03455181,0.0024264536,0.05855943,0.054163553],"study_design_scores_gemma":[0.000038723025,0.00003973867,0.97282505,0.00001512673,0.000033837885,0.00010712775,0.000054944114,0.0044570337,0.0050751218,0.0004006297,0.016927514,0.00002512221],"about_ca_topic_score_codex":0.0118425805,"about_ca_topic_score_gemma":0.025035243,"teacher_disagreement_score":0.0118425805,"about_ca_system_score_codex":0.00033126443,"about_ca_system_score_gemma":0.00030752606,"threshold_uncertainty_score":0.023547292},"labels":[],"label_agreement":null},{"id":"W2728399314","doi":"10.3847/1538-4357/aa7da6","title":"Simultaneous Monitoring of X-Ray and Radio Variability in Sagittarius A*","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; McGill University","funders":"","keywords":"Astrophysics; Flare; Physics; Sagittarius A*; Millimeter; Wavelength; X-ray; Astronomy; Supermassive black hole; Optics","score_opus":0.013697146880576425,"score_gpt":0.25164436312044586,"score_spread":0.23794721623986942,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2728399314","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843127,0.000071319,0.0003112437,0.000014736833,0.000004894356,0.000006147381,0.00031325346,0.000038710146,0.00080834515],"genre_scores_gemma":[0.9982127,0.00003590643,0.0005277445,0.000021475415,0.000012804455,0.000008263268,0.00094809564,0.000011714884,0.00022133939],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998759,0.000016240507,0.0000106559055,0.00004415137,0.000031931322,0.000021077778],"domain_scores_gemma":[0.9995634,0.000034012544,0.00016625557,0.00004268587,0.0000805843,0.000113129325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002616422,0.00019906161,0.00021760665,0.0010380484,0.0003151366,0.00050380046,0.00023016873,0.0002205891,0.0007140277],"category_scores_gemma":[0.0003229432,0.00012612292,0.00022332564,0.00054805755,0.0001804537,0.0002371093,0.00047143447,0.0002108523,0.00027852817],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023177355,0.00009295372,0.8794676,0.000039526734,0.00019684703,0.00023912218,0.00022282879,0.0005708144,0.104237475,0.00007725443,0.00030590346,0.01431795],"study_design_scores_gemma":[0.000003046791,0.00006945776,0.99791104,0.0000023333062,0.0000132171635,0.000084173604,0.000045148176,0.0003416041,0.0010642718,0.000021078831,0.0004408779,0.0000037379407],"about_ca_topic_score_codex":0.003933434,"about_ca_topic_score_gemma":0.005788915,"teacher_disagreement_score":0.003933434,"about_ca_system_score_codex":0.00021087762,"about_ca_system_score_gemma":0.00014264618,"threshold_uncertainty_score":0.007821083},"labels":[],"label_agreement":null},{"id":"W2728850873","doi":"10.3847/1538-4357/aa7c5f","title":"Hubble Space Telescope Proper Motion (HSTPROMO) Catalogs of Galactic Globular Clusters. V. The Rapid Rotation of 47 Tuc Traced and Modeled in Three Dimensions<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Physics; Rotation (mathematics); Astrophysics; Proper motion; Differential rotation; Cluster (spacecraft); Surface brightness; Kinematics; Galaxy; Geometry; Classical mechanics; Stars","score_opus":0.014204447575960389,"score_gpt":0.22675460748151857,"score_spread":0.21255015990555817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2728850873","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9222835,0.00080869,0.0019356691,0.000093847215,0.000027056467,0.000047152902,0.0695467,0.0007556454,0.004501789],"genre_scores_gemma":[0.8701922,0.00052547106,0.003715157,0.000036949175,0.000043414744,0.000041396546,0.12349384,0.0000917338,0.0018597286],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999107,0.000005787333,0.000005367856,0.000026677873,0.000025047566,0.000026469332],"domain_scores_gemma":[0.99971193,0.000019746996,0.00008646967,0.0000636648,0.00005594061,0.00006223806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001818386,0.00023376578,0.00017805792,0.0021900919,0.00029251346,0.0004772823,0.00026465714,0.00025211365,0.0013216082],"category_scores_gemma":[0.0005152691,0.00008479827,0.00028002614,0.0020252543,0.00014572925,0.00022262281,0.00037065946,0.00012197089,0.0009967354],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002717182,0.00003960063,0.8803172,0.00017291732,0.00015300585,0.0004319622,0.00038009588,0.011622485,0.014813426,0.0026209292,0.024932697,0.064243875],"study_design_scores_gemma":[0.000007697339,0.000019861518,0.97770226,0.000021738204,0.000024598457,0.00013804756,0.00010450859,0.0061318437,0.0014363555,0.00024371406,0.014159194,0.000010179197],"about_ca_topic_score_codex":0.038359474,"about_ca_topic_score_gemma":0.044870857,"teacher_disagreement_score":0.038359474,"about_ca_system_score_codex":0.000624553,"about_ca_system_score_gemma":0.0005085092,"threshold_uncertainty_score":0.07627237},"labels":[],"label_agreement":null},{"id":"W2728892570","doi":"10.3847/1538-4357/aa8b17","title":"Importance of Resolving the Spectral Support of Beam-plasma Instabilities in Simulations","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Laser-Plasma Interactions and Diagnostics","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Plasma; Beam (structure); Instability; Astrophysics; Computational physics; Astronomy; Optics; Mechanics; Nuclear physics","score_opus":0.014999713998802955,"score_gpt":0.2715561059484919,"score_spread":0.25655639194968893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2728892570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9165291,0.0004821165,0.06562586,0.001775282,0.00023564477,0.00024678832,0.00083203055,0.001119059,0.013154056],"genre_scores_gemma":[0.97416556,0.00013646475,0.024201648,0.00018324626,0.000027441223,0.00021978187,0.00024228425,0.00017200444,0.0006516202],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999337,0.0003286993,0.00005159597,0.000058383484,0.00012685874,0.00009742972],"domain_scores_gemma":[0.9872248,0.01070099,0.0004103474,0.000735824,0.00061203045,0.0003159408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023910427,0.00083792553,0.0012066845,0.00056529645,0.00095447665,0.0014424936,0.0013749079,0.0015768561,0.0022604666],"category_scores_gemma":[0.018834177,0.0006007084,0.00048831705,0.00044249656,0.0011541146,0.0017916767,0.000951048,0.0019039976,0.00029230828],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018815849,0.0002746956,0.006124251,0.0001263234,0.0000625679,0.000116615876,0.00016015167,0.97699183,0.0054992326,0.005135086,0.0005614555,0.0047595343],"study_design_scores_gemma":[0.000021570608,0.0000313167,0.00046473957,0.000018962866,0.000012229168,0.000009593558,0.000036913254,0.9965707,0.0017773585,0.0007820065,0.0002639326,0.0000105729505],"about_ca_topic_score_codex":0.010324498,"about_ca_topic_score_gemma":0.008202417,"teacher_disagreement_score":0.010324498,"about_ca_system_score_codex":0.00066997716,"about_ca_system_score_gemma":0.0018035724,"threshold_uncertainty_score":0.020528853},"labels":[],"label_agreement":null},{"id":"W2729177279","doi":"10.3847/1538-4357/aa7d0d","title":"Galaxy Formation through Filamentary Accretion at z = 6.1","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Accretion (finance); Lenticular galaxy; Galaxy merger; Interacting galaxy; Type-cD galaxy; Irregular galaxy; Astronomy; Galaxy formation and evolution","score_opus":0.013312726303651339,"score_gpt":0.23853820031459982,"score_spread":0.22522547401094847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2729177279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99786407,0.00009068963,0.00034880295,0.000030106581,0.0000017282548,0.0000027645629,0.00022077307,0.000039245904,0.0014017723],"genre_scores_gemma":[0.9992901,0.000023899322,0.00023338651,0.0000068804648,0.0000029636908,0.0000010492911,0.00025806765,0.000002480714,0.00018110721],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995065,0.00000381229,0.0000019547465,0.000013695043,0.000010132066,0.000019799369],"domain_scores_gemma":[0.99981505,0.00001501088,0.00007868815,0.000021059677,0.000015799707,0.000054362103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010501248,0.000121569705,0.00012540913,0.00039683463,0.00022554383,0.00053091015,0.00026831243,0.00015828779,0.0014502115],"category_scores_gemma":[0.00026174722,0.000117382944,0.00017030007,0.0002786344,0.00017214064,0.0002626056,0.0004033427,0.0001865044,0.00021557993],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003553121,0.00007101703,0.91396815,0.000045055625,0.0001193026,0.00059705996,0.0005878909,0.0033569292,0.061665654,0.002876257,0.0009696501,0.015387635],"study_design_scores_gemma":[0.000007219128,0.0000264165,0.9939779,0.0000056027206,0.00001222403,0.00011016683,0.00003726631,0.002437496,0.0020084016,0.00050265784,0.0008713921,0.000003232294],"about_ca_topic_score_codex":0.0037635502,"about_ca_topic_score_gemma":0.002444618,"teacher_disagreement_score":0.0037635502,"about_ca_system_score_codex":0.00038592267,"about_ca_system_score_gemma":0.00006481828,"threshold_uncertainty_score":0.0074833035},"labels":[],"label_agreement":null},{"id":"W2730555596","doi":"10.3847/1538-4357/aa7c1c","title":"Evidence for Spatially Correlated Gaia Parallax Errors in the Kepler Field","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Leibniz-Gemeinschaft; Science Mission Directorate; Max-Planck-Institut für Astronomie; York University; New Mexico State University; University of Notre Dame; Carnegie Mellon University; Office of Science; Johns Hopkins University; University of Utah; Ohio State University; Carnegie Institution of Washington; Smithsonian Institution; Alfred P. Sloan Foundation; Max-Planck-Institut für Astrophysik; U.S. Department of Energy; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Parallax; Kepler; Astronomy; Astrophysics; Field (mathematics); Astrometry; Stars","score_opus":0.04790605558995087,"score_gpt":0.2990901600319831,"score_spread":0.2511841044420322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2730555596","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99636793,0.00012990116,0.0017169593,0.000041462717,0.0000056719123,0.0000038705352,0.00028091477,0.00004059183,0.0014127215],"genre_scores_gemma":[0.99961555,0.000010476313,0.0001684556,0.0000058504806,0.000002872917,0.0000017969788,0.00009986682,0.000008751685,0.000086262095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99773514,0.00059116905,0.00017004347,0.0008879376,0.00045508708,0.00016056276],"domain_scores_gemma":[0.9746026,0.007079755,0.009188506,0.005359565,0.0032864,0.00048324527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002093906,0.00028707707,0.00044930045,0.0019080807,0.0004145992,0.0011241196,0.00048003494,0.00032815506,0.001032987],"category_scores_gemma":[0.014513343,0.00032808498,0.00028809565,0.0017063104,0.0010106099,0.00083833846,0.0011882342,0.00033214194,0.00037526488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008854147,0.000009458078,0.9889459,0.000014676113,0.00009316253,0.00004712494,0.00039083546,0.0011761574,0.0041078147,0.0006431517,0.00013150171,0.0043518343],"study_design_scores_gemma":[0.000004339789,0.000023613067,0.9966479,0.0000067163683,0.000024166902,0.0000629369,0.00014190491,0.0013493501,0.0010477111,0.00043031925,0.00025213248,0.000008987913],"about_ca_topic_score_codex":0.006423356,"about_ca_topic_score_gemma":0.007591522,"teacher_disagreement_score":0.006423356,"about_ca_system_score_codex":0.00054051547,"about_ca_system_score_gemma":0.00028645014,"threshold_uncertainty_score":0.0127719045},"labels":[],"label_agreement":null},{"id":"W2730727805","doi":"10.3847/1538-4357/aa7c60","title":"The TWA 3 Young Triple System: Orbits, Disks, Evolution","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Astrophysics Division; National Aeronautics and Space Administration; California Institute of Technology; U.S. Naval Observatory; W. M. Keck Foundation; University of Toledo; Northern Arizona University; Yale University; National Science Foundation","keywords":"Circumbinary planet; Physics; Spectroscopy; Astrophysics; Binary number; Mass ratio; Orbit (dynamics); Eccentricity (behavior); Orbital period; Orbital inclination; Orbital elements; Orbital eccentricity; Confusion; Astronomy; Stars; Mathematics","score_opus":0.010691036739630273,"score_gpt":0.2307777457769102,"score_spread":0.22008670903727995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2730727805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972058,0.00034648005,0.0007733334,0.000045879482,0.000008516071,0.000011330028,0.00030223103,0.000040665076,0.0012656321],"genre_scores_gemma":[0.99806553,0.00004081885,0.0009750401,0.000022956354,0.000009124025,0.0000063903685,0.00054937956,0.000015186832,0.00031548904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990726,0.0000069580474,0.000005496343,0.000030422472,0.000024438617,0.00002538799],"domain_scores_gemma":[0.9995403,0.00003138343,0.00014553782,0.000048899878,0.00006133851,0.00017260872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002726938,0.00025665553,0.00030090596,0.0009667579,0.0013215087,0.00090381916,0.00032436132,0.00042207516,0.0015257478],"category_scores_gemma":[0.00041789084,0.0001850164,0.00021387267,0.0008064305,0.00033704002,0.000560974,0.0008238519,0.00046082307,0.00075865886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039070757,0.0002029295,0.844619,0.00006998057,0.00009277809,0.00084249536,0.0007625461,0.0016389166,0.11623003,0.002182759,0.0013145218,0.0316534],"study_design_scores_gemma":[0.000028544304,0.0002911269,0.9657705,0.000028386907,0.000049397095,0.0028129276,0.00066740863,0.012536465,0.008904117,0.0026949306,0.0061774054,0.000038929695],"about_ca_topic_score_codex":0.002636022,"about_ca_topic_score_gemma":0.0036767914,"teacher_disagreement_score":0.002636022,"about_ca_system_score_codex":0.00061235676,"about_ca_system_score_gemma":0.00028910078,"threshold_uncertainty_score":0.0052413344},"labels":[],"label_agreement":null},{"id":"W2732529634","doi":"10.3847/1538-4357/aaf390","title":"The Effect of Carbon Grain Destruction on the Chemical Structure of Protoplanetary Disks","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Korea Astronomy and Space Science Institute; Yukawa Institute for Theoretical Physics, Kyoto University; National Research Foundation of Korea; National Research Foundation; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Queen's University; University of Leeds; Academia Sinica; Japan Society for the Promotion of Science; Queen's University Belfast; Ministry of Education, Culture, Sports, Science and Technology","keywords":"Protoplanetary disk; Astrobiology; Carbon fibers; Planetesimal; Astrophysics; Geology; Materials science; Physics; Solar System; Planet; Composite material","score_opus":0.0026818581287387597,"score_gpt":0.18776375031784245,"score_spread":0.1850818921891037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2732529634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99902725,0.000052080894,0.00027886397,0.000016845323,0.0000017439565,0.0000011041044,0.00007261162,0.000014149096,0.0005352672],"genre_scores_gemma":[0.99976784,0.000014421037,0.00006972837,0.0000030251006,4.7469146e-7,5.877089e-7,0.00004153467,0.0000035383268,0.00009884536],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994576,0.000008999184,0.000002348267,0.000013121736,0.000013852391,0.000015938183],"domain_scores_gemma":[0.9995827,0.00018944083,0.000079004734,0.000045394747,0.000042223553,0.000061306964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012119654,0.0002506717,0.00015457738,0.0002642381,0.00021327559,0.00029624676,0.00031262654,0.00026522778,0.0011028433],"category_scores_gemma":[0.0006781501,0.0001293936,0.00023462431,0.00014419522,0.00030297888,0.0002132213,0.00017986604,0.00017073321,0.00015549528],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001156005,0.00015824534,0.30635044,0.0000888638,0.00023028225,0.0006003048,0.00006622308,0.522862,0.1586298,0.0015064398,0.0003920653,0.007959262],"study_design_scores_gemma":[0.00009081282,0.00032699615,0.3580431,0.000008277418,0.00011180953,0.000292207,0.00014164274,0.53253394,0.10639959,0.0010626266,0.0009653804,0.000023576975],"about_ca_topic_score_codex":0.0038956422,"about_ca_topic_score_gemma":0.002181154,"teacher_disagreement_score":0.0038956422,"about_ca_system_score_codex":0.00050827325,"about_ca_system_score_gemma":0.00011347532,"threshold_uncertainty_score":0.0077459216},"labels":[],"label_agreement":null},{"id":"W2732921053","doi":"10.3847/1538-4357/aa7e89","title":"Formation of Double Neutron Star Systems","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":689,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Neutron star; Astronomy; Astrophysics; Nuclear physics","score_opus":0.023163775632316228,"score_gpt":0.330391040102552,"score_spread":0.30722726447023574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2732921053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938877,0.00012807723,0.0024175353,0.000022571448,0.000013612916,0.000012212888,0.00003868193,0.00002687047,0.0034527828],"genre_scores_gemma":[0.9976477,0.000051107465,0.0015883866,0.0000088379375,0.0000032019332,0.0000068917807,0.00010395274,0.0000069984417,0.00058284623],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998684,0.000020480922,0.000008740534,0.000043913402,0.000029943198,0.000028603434],"domain_scores_gemma":[0.99961036,0.000064890235,0.00011100463,0.000044524753,0.00004206949,0.00012717946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022618343,0.00019463952,0.0003199595,0.00045265447,0.0007183206,0.0010538524,0.00037474808,0.00032755212,0.0018447312],"category_scores_gemma":[0.0010128336,0.00022623237,0.00035763436,0.0001947253,0.0005143071,0.0005902712,0.0010947739,0.00027357347,0.00019934349],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061605335,0.0003860266,0.38373795,0.00042777936,0.00040810386,0.00416569,0.0017661785,0.32545835,0.13279755,0.103915334,0.0020928143,0.044228237],"study_design_scores_gemma":[0.00016118289,0.0010314465,0.17789124,0.000113108654,0.00017020995,0.0037533394,0.0012036732,0.7037291,0.06383567,0.029936675,0.018039307,0.00013501864],"about_ca_topic_score_codex":0.00097041746,"about_ca_topic_score_gemma":0.00091057434,"teacher_disagreement_score":0.0018447312,"about_ca_system_score_codex":0.0005501599,"about_ca_system_score_gemma":0.00028621402,"threshold_uncertainty_score":0.0061712265},"labels":[],"label_agreement":null},{"id":"W2733266992","doi":"10.3847/1538-4357/aa77f9","title":"The 9577 and 9632 Å Diffuse Interstellar Bands: as Carrier","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Spectral line; Astrophysics; Absorption spectroscopy; Astronomical spectroscopy; Interstellar medium; Stellar atmosphere; Absorption (acoustics); Atmosphere (unit); Atomic physics; Astronomy; Optics; Galaxy","score_opus":0.009141893501064752,"score_gpt":0.21824361028849742,"score_spread":0.20910171678743267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2733266992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9765953,0.0015342364,0.0059785177,0.0002359713,0.00010812541,0.000018924688,0.000676943,0.00017530864,0.014676565],"genre_scores_gemma":[0.9971896,0.00008966034,0.00091052573,0.000029130722,0.000008841583,0.00000375297,0.00028103328,0.000022033948,0.0014654498],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9996437,0.000026435071,0.000015199709,0.00015775402,0.000087183056,0.000069616195],"domain_scores_gemma":[0.99955016,0.000040956013,0.00012339404,0.00009816275,0.000115021714,0.00007229872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003459911,0.00048787083,0.00027691777,0.0009265305,0.00047162734,0.0013433971,0.000880511,0.00040687495,0.0051907324],"category_scores_gemma":[0.0006379411,0.00015867026,0.00020484296,0.001382904,0.00039963497,0.0009554251,0.00074560574,0.0004239599,0.0011401497],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013178783,0.00024803533,0.33135927,0.0003550134,0.0003274488,0.001390549,0.00078416755,0.004014622,0.5193673,0.022755502,0.005027374,0.11305286],"study_design_scores_gemma":[0.0001497319,0.00054033136,0.5613299,0.00015217517,0.0003341573,0.0025018323,0.0016925338,0.023513358,0.32927614,0.011093117,0.06931351,0.00010319907],"about_ca_topic_score_codex":0.002564525,"about_ca_topic_score_gemma":0.0019326076,"teacher_disagreement_score":0.0051907324,"about_ca_system_score_codex":0.00058372784,"about_ca_system_score_gemma":0.0002605079,"threshold_uncertainty_score":0.01736474},"labels":[],"label_agreement":null},{"id":"W2733871128","doi":"10.3847/1538-4357/aa94c7","title":"Tidal Disruption Event Host Galaxies in the Context of the Local Galaxy Population","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Galaxy; Bulge; Peculiar galaxy; Context (archaeology); Galaxy merger; Elliptical galaxy; Luminous infrared galaxy; Population; Galaxy formation and evolution","score_opus":0.009238329366953502,"score_gpt":0.2390513798412205,"score_spread":0.22981305047426698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2733871128","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991978,0.00008616579,0.00005923325,0.000018984914,8.036829e-7,0.0000013654089,0.00028360818,0.0000052522587,0.00034689],"genre_scores_gemma":[0.99953365,0.000029929206,0.00002700979,0.0000048940724,0.000002778402,8.140266e-7,0.0002932639,0.0000027224032,0.0001049658],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965227,0.00006973334,0.000022146218,0.00011857312,0.000051437364,0.00008573945],"domain_scores_gemma":[0.99677294,0.0007088756,0.0012482798,0.0003618639,0.00038044326,0.0005275352],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045802922,0.00011605084,0.00030410898,0.0016895111,0.0003881712,0.0010989357,0.00028418557,0.0002132455,0.0022256752],"category_scores_gemma":[0.0028574048,0.00009108884,0.00021577942,0.0018483909,0.00059794623,0.0006278771,0.00076009234,0.00021010393,0.00038812088],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002383773,0.0000062378895,0.99793696,0.0000052087717,0.000030059835,0.00004617571,0.00011555863,0.00021617481,0.00046736974,0.00008102683,0.0000855596,0.0009858524],"study_design_scores_gemma":[7.6304946e-7,0.000008890772,0.9992091,0.0000012005644,0.000007872761,0.00005234429,0.00018053435,0.00032004918,0.00006396681,0.000028168854,0.0001252603,0.000001771825],"about_ca_topic_score_codex":0.016047357,"about_ca_topic_score_gemma":0.023358503,"teacher_disagreement_score":0.016047357,"about_ca_system_score_codex":0.0004137109,"about_ca_system_score_gemma":0.00014959143,"threshold_uncertainty_score":0.031907916},"labels":[],"label_agreement":null},{"id":"W2734432583","doi":"10.3847/1538-4357/aa8035","title":"The Origins of [C ii] Emission in Local Star-forming Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Interstellar medium; Metallicity; Ionization; Galaxy; Emission spectrum; Line (geometry); Photoelectric effect; Plasma","score_opus":0.01217085273554232,"score_gpt":0.2629777216555267,"score_spread":0.2508068689199844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2734432583","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953115,0.000071819806,0.000037571164,0.000003681699,3.7609487e-7,0.0000016484744,0.000095473646,0.000005945994,0.00025240247],"genre_scores_gemma":[0.9997613,0.000019678504,0.000036594873,0.0000040681566,9.773814e-7,0.0000011706998,0.00012695351,0.0000017770648,0.00004758941],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983335,0.000015885389,0.000008011738,0.00007300231,0.000026296048,0.000043369575],"domain_scores_gemma":[0.9994413,0.000059590748,0.00021825595,0.000043988264,0.000063457555,0.00017334399],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018291449,0.00023621238,0.00023646001,0.0013184933,0.00031445327,0.0005750004,0.00033833116,0.00024179352,0.001052146],"category_scores_gemma":[0.0004936991,0.00016040151,0.00017667438,0.0006501355,0.00046098675,0.00025364343,0.00039618692,0.00011588784,0.00028336202],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000064505686,0.000015620846,0.9839632,0.000011808462,0.00004440147,0.00004633365,0.00023428175,0.00011914585,0.013801272,0.000055680557,0.000053809672,0.0015899421],"study_design_scores_gemma":[9.127926e-7,0.000009298861,0.9995103,0.000001299916,0.0000039088613,0.000023819752,0.0000704745,0.000080423175,0.00023894687,0.000010991355,0.000048390015,0.0000012850263],"about_ca_topic_score_codex":0.007863567,"about_ca_topic_score_gemma":0.010822363,"teacher_disagreement_score":0.007863567,"about_ca_system_score_codex":0.00044528424,"about_ca_system_score_gemma":0.00009500491,"threshold_uncertainty_score":0.01563561},"labels":[],"label_agreement":null},{"id":"W2734692244","doi":"10.3847/1538-4357/aa7fe9","title":"ALMA Observations of Dust Polarization and Molecular Line Emission from the Class 0 Protostellar Source Serpens SMM1","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Ministerio de Educación, Cultura y Deporte; Koninklijke Nederlandse Akademie van Wetenschappen; European Commission; Gordon and Betty Moore Foundation; National Science Foundation; James S. McDonnell Foundation; National Aeronautics and Space Administration","keywords":"Serpens; Physics; Astrophysics; Protostar; Astronomy; Polarization (electrochemistry); Emission spectrum; Molecular cloud; Line (geometry); Stars; Spectral line; Star formation","score_opus":0.019249852513589103,"score_gpt":0.24892279906722095,"score_spread":0.22967294655363185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2734692244","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99870384,0.00003076991,0.000092504095,0.000011496669,0.0000022858917,0.000002447096,0.0002964965,0.000025453988,0.00083481707],"genre_scores_gemma":[0.998735,0.000030435735,0.00037760037,0.0000113493725,0.000008164246,0.0000032079793,0.000642394,0.00000541195,0.0001864815],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994826,0.0000057241073,0.000002038336,0.000016090655,0.000016234804,0.000011647381],"domain_scores_gemma":[0.99985194,0.000017425862,0.000049335125,0.000018157463,0.000020342046,0.000042742886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009832614,0.00016631893,0.00013359339,0.00067414326,0.00025462208,0.0002292375,0.0002064778,0.00013676118,0.0010567079],"category_scores_gemma":[0.00024729795,0.00009836993,0.00012156681,0.00027935047,0.00010974358,0.00012495398,0.000288844,0.00015222958,0.0002571822],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044785027,0.00010570028,0.7872243,0.000059079073,0.00008762778,0.0007835604,0.00050209806,0.0011323424,0.18052603,0.0003020566,0.0011233515,0.02770603],"study_design_scores_gemma":[0.000010478524,0.000043555297,0.99479324,0.0000056733375,0.000009953429,0.0001472663,0.000073860996,0.0008954261,0.0030268915,0.00003909611,0.0009508781,0.0000036946806],"about_ca_topic_score_codex":0.0022876651,"about_ca_topic_score_gemma":0.004742955,"teacher_disagreement_score":0.0022876651,"about_ca_system_score_codex":0.0001995226,"about_ca_system_score_gemma":0.00007688319,"threshold_uncertainty_score":0.0045487285},"labels":[],"label_agreement":null},{"id":"W2735092754","doi":"10.3847/1538-4357/aa8dfb","title":"Constraints on Galactic Neutrino Emission with Seven Years of IceCube Data","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Snolab; University of Alberta","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Western Canada Research Grid; Vlaamse regering; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Neutrino; Galactic plane; Astrophysics; Flux (metallurgy); Cosmic ray; Astronomy; Neutrino astronomy; Muon; Neutrino detector; Galaxy; Neutrino oscillation; Nuclear physics","score_opus":0.02091442152365881,"score_gpt":0.2615242895178854,"score_spread":0.24060986799422662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2735092754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95593274,0.00089445943,0.011590809,0.0003540126,0.000044047836,0.00009819861,0.021944596,0.00033597616,0.008805053],"genre_scores_gemma":[0.93233556,0.00041673778,0.011301336,0.00018132458,0.00005052706,0.00017586653,0.054770038,0.00014815704,0.00062053965],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9979139,0.00080369087,0.00017597995,0.0003812345,0.00044318082,0.0002821126],"domain_scores_gemma":[0.990593,0.0052792337,0.0014071867,0.0013250624,0.0009880129,0.00040750636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0044909697,0.0007780649,0.00087684306,0.0013076887,0.00058382575,0.0020256785,0.00083868834,0.0009052119,0.0016009681],"category_scores_gemma":[0.01073012,0.0003992399,0.0010054182,0.0016793701,0.00043953425,0.0008201247,0.0010014857,0.00056687323,0.0004646161],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0032801528,0.00030910104,0.70781785,0.00040994835,0.001459698,0.00064453285,0.0004950555,0.22426924,0.010664907,0.009917592,0.008130376,0.03260157],"study_design_scores_gemma":[0.000613392,0.00060637767,0.5257257,0.00043474112,0.00062163186,0.0006364955,0.00063609926,0.33571193,0.037918705,0.01498453,0.081802204,0.000308245],"about_ca_topic_score_codex":0.010237835,"about_ca_topic_score_gemma":0.011724516,"teacher_disagreement_score":0.010237835,"about_ca_system_score_codex":0.00076501153,"about_ca_system_score_gemma":0.00070107385,"threshold_uncertainty_score":0.023750782},"labels":[],"label_agreement":null},{"id":"W2735212190","doi":"10.3847/1538-4357/aab3ca","title":"First Observation of the Submillimeter Polarization Spectrum in a Translucent Molecular Cloud","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Polarization (electrochemistry); Cosmic microwave background; Polarimetry; Molecular cloud; Polarization in astronomy; Cosmic dust; Observable; Infrared; Degree of polarization","score_opus":0.009959610975267458,"score_gpt":0.21575363401606812,"score_spread":0.20579402304080066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2735212190","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932753,0.00020685428,0.0025441414,0.00013336437,0.000024100473,0.000014190167,0.000961472,0.00011703752,0.002723499],"genre_scores_gemma":[0.99787056,0.000040935334,0.0013778592,0.000067336405,0.000019185165,0.0000036716651,0.00042855722,0.000016383765,0.00017545937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999879,0.0000064920823,0.0000023714722,0.000043149266,0.000034380704,0.000034608114],"domain_scores_gemma":[0.9997131,0.000053075924,0.000060726914,0.00004179547,0.00006597844,0.00006519192],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016089753,0.00020169685,0.00021230032,0.00050410547,0.000646528,0.0005508024,0.00032917655,0.0003117753,0.0009311018],"category_scores_gemma":[0.00022050712,0.00021516246,0.00019988306,0.00040286352,0.00033489038,0.00023407867,0.0004158651,0.00065371336,0.000297161],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006467595,0.00026259766,0.49608883,0.0001033707,0.0002063619,0.003111062,0.00067875325,0.001907947,0.4584957,0.0016294203,0.004018097,0.03285113],"study_design_scores_gemma":[0.000030852956,0.0002001558,0.9526938,0.000024962166,0.00007035235,0.0010969191,0.00021306676,0.0062006796,0.031496078,0.00059910037,0.007343625,0.000030315878],"about_ca_topic_score_codex":0.0030437214,"about_ca_topic_score_gemma":0.0039887303,"teacher_disagreement_score":0.0030437214,"about_ca_system_score_codex":0.0003188842,"about_ca_system_score_gemma":0.00012899937,"threshold_uncertainty_score":0.006052017},"labels":[],"label_agreement":null},{"id":"W2735235936","doi":"","title":"Space Telescope and Optical Reverberation Mapping Project. VI. Reverberating Disk Models for NGS 5548","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Western University","funders":"","keywords":"Physics; Light curve; Astrophysics; Reverberation mapping; Astronomy; RADIUS; Black-body radiation; Accretion (finance); Spectral line; Accretion disc; Galaxy; Wavelength; Active galactic nucleus; Angstrom; Radiation; Optics","score_opus":0.032392389995737084,"score_gpt":0.2713658630924418,"score_spread":0.23897347309670475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2735235936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94301766,0.00028636467,0.041496534,0.00052199245,0.00004989611,0.000095169155,0.0031750733,0.00069915724,0.010658136],"genre_scores_gemma":[0.98177207,0.00012233447,0.011888945,0.00006943478,0.000035184945,0.000075511896,0.0016199747,0.00013496596,0.004281547],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993503,0.000020783697,0.0000026495975,0.00001844803,0.000011371313,0.000011819887],"domain_scores_gemma":[0.9998385,0.000027583194,0.000040808416,0.00003783026,0.000025247995,0.00002999918],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032521036,0.0004374134,0.00032819418,0.00046635303,0.00022976659,0.0003973826,0.0010568892,0.0005332324,0.002916432],"category_scores_gemma":[0.0008245906,0.0001962354,0.000470703,0.00030335318,0.00018197579,0.0004527207,0.00036075045,0.0002555382,0.0007307217],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002803291,0.00015205398,0.06348757,0.00006657651,0.00012291674,0.0006960368,0.00037531578,0.87703854,0.0067557613,0.014845973,0.009455557,0.026723377],"study_design_scores_gemma":[0.000050240888,0.00003862325,0.009893598,0.000006252063,0.000013745551,0.00009283713,0.000034165252,0.98146975,0.00029828394,0.005096748,0.002992701,0.000013220896],"about_ca_topic_score_codex":0.018098963,"about_ca_topic_score_gemma":0.01074232,"teacher_disagreement_score":0.018098963,"about_ca_system_score_codex":0.000726893,"about_ca_system_score_gemma":0.0002884942,"threshold_uncertainty_score":0.0359872},"labels":[],"label_agreement":null},{"id":"W2735566531","doi":"10.3847/1538-4357/aa88ca","title":"Buried AGNs in Advanced Mergers: Mid-infrared Color Selection as a Dual AGN Candidate Finder","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Galaxy; Active galactic nucleus; Supermassive black hole; Galaxy merger; Population; Optical spectra; Galaxy formation and evolution","score_opus":0.007852200499691,"score_gpt":0.24108642487488288,"score_spread":0.23323422437519187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2735566531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988404,0.000119434415,0.00041455988,0.000028764785,0.0000037919417,0.0000070389838,0.00004354414,0.000024434086,0.00051809516],"genre_scores_gemma":[0.9992175,0.000025076457,0.0005391193,0.000017903518,0.000007953439,0.0000017146325,0.00006941392,0.0000026350208,0.00011863713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978775,0.000029892908,0.000015497635,0.000052364816,0.00006079594,0.000053709315],"domain_scores_gemma":[0.9992176,0.00010753747,0.00028288123,0.000048726026,0.00008461377,0.00025862962],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046522325,0.000218564,0.00024261027,0.0016900533,0.00043616618,0.00070871104,0.0003755827,0.0002621041,0.001076593],"category_scores_gemma":[0.000635903,0.00014412732,0.00015595052,0.00048948,0.00032152605,0.0003123608,0.0006314965,0.00030413418,0.0002676749],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016209568,0.00006337807,0.96536595,0.000011154646,0.00001609078,0.0009321047,0.00027348808,0.00008349144,0.025807677,0.00011773899,0.00017740527,0.006989456],"study_design_scores_gemma":[0.000006067954,0.00011632896,0.9916819,0.0000057393886,0.00002004218,0.003192275,0.00030304075,0.0009180911,0.0031204307,0.000119154996,0.00050911464,0.000007933948],"about_ca_topic_score_codex":0.00072851125,"about_ca_topic_score_gemma":0.0013784684,"teacher_disagreement_score":0.0016900533,"about_ca_system_score_codex":0.00014217255,"about_ca_system_score_gemma":0.00009863632,"threshold_uncertainty_score":0.0036014915},"labels":[],"label_agreement":null},{"id":"W2735775808","doi":"10.3847/1538-4357/aa7842","title":"Erratum: “Cloud Structure of Three Galactic Infrared Dark Star-forming Regions from Combining Ground and Space-based Bolometric Observations” (2017, ApJ, 840, 22)","year":2017,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Bolometer; Molecular cloud; Astronomy; Infrared; Stars; Detector","score_opus":0.0295406269784125,"score_gpt":0.2498246120767111,"score_spread":0.2202839850982986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2735775808","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0016486421,0.000892843,0.00040933,0.0377702,0.946413,0.00003112749,0.006496572,0.0004013516,0.0059369965],"genre_scores_gemma":[0.04292686,0.0077433693,0.0066984203,0.0986708,0.29700297,0.00022621328,0.044347987,0.003114615,0.4992687],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9990434,0.0000632935,0.00020874677,0.00015371323,0.0004334207,0.00009740455],"domain_scores_gemma":[0.99339175,0.0009322808,0.00050071336,0.0004736572,0.0042564007,0.00044528238],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011389089,0.0015755947,0.0009997088,0.0027159902,0.0027108274,0.0024636737,0.0021641129,0.002712567,0.042052697],"category_scores_gemma":[0.013729324,0.00058987073,0.0009948285,0.0018482212,0.0010602226,0.001926652,0.0017325983,0.0038741026,0.026809288],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043994645,0.000009690958,0.00039555648,0.000059120248,0.000008984905,0.000179995,0.000015930325,0.000041277744,0.00011397411,0.0002601095,0.9955146,0.0033568281],"study_design_scores_gemma":[0.000082080274,0.00005379589,0.012031881,0.0002943413,0.00008056919,0.0006734258,0.0003024927,0.0004400521,0.0010048387,0.0014540483,0.98350483,0.000077518256],"about_ca_topic_score_codex":0.03015163,"about_ca_topic_score_gemma":0.03823347,"teacher_disagreement_score":0.042052697,"about_ca_system_score_codex":0.0020425965,"about_ca_system_score_gemma":0.0037944068,"threshold_uncertainty_score":0.14068025},"labels":[],"label_agreement":null},{"id":"W2735822899","doi":"10.3847/1538-4357/aa7894","title":"Distances to Supernova Remnants G31.9+0.0 and G54.4−0.3 Associated with Molecular Clouds","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Supernova; Molecular cloud; Astrophysics; Supernova remnant; Absorption (acoustics); Spectral line; Absorption spectroscopy; Noise (video); Astronomy; Stars; Optics; Image (mathematics); Artificial intelligence","score_opus":0.008565624734014322,"score_gpt":0.23131149913986304,"score_spread":0.22274587440584873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2735822899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979353,0.0001947719,0.000237411,0.00004757276,0.000016278917,0.0000039677684,0.0003212327,0.00003614912,0.0012074002],"genre_scores_gemma":[0.99816614,0.00010455084,0.0004365266,0.000016283146,0.0000145549175,0.000003846286,0.00079685345,0.000009346113,0.00045199724],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972993,0.000018413279,0.000029013192,0.000093892544,0.000071850256,0.000056931276],"domain_scores_gemma":[0.9980202,0.00020218552,0.00064540637,0.00024109798,0.00031468717,0.0005763883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055289484,0.00033976242,0.00033405842,0.002171058,0.00057046633,0.0007924349,0.000537178,0.00040902084,0.0024282709],"category_scores_gemma":[0.0011312185,0.00020114318,0.0005253695,0.0008868876,0.00066798384,0.00053145067,0.0011351304,0.00041590314,0.00077348883],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004976769,0.000036839898,0.96673244,0.000035847024,0.00017380896,0.0004240867,0.00034597868,0.0005765843,0.02068534,0.0008166646,0.00049393915,0.009180869],"study_design_scores_gemma":[0.00001107306,0.000050535735,0.9971052,0.00000393788,0.000027134472,0.00030940038,0.000074407435,0.00016584067,0.0010709108,0.00020174256,0.0009701982,0.000009623598],"about_ca_topic_score_codex":0.006532599,"about_ca_topic_score_gemma":0.009322485,"teacher_disagreement_score":0.006532599,"about_ca_system_score_codex":0.0007601399,"about_ca_system_score_gemma":0.00019670786,"threshold_uncertainty_score":0.012989163},"labels":[],"label_agreement":null},{"id":"W2736479339","doi":"10.3847/1538-4357/aa80e5","title":"The JCMT BISTRO Survey: The Magnetic Field Strength in the Orion A Filament","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec; Western University","funders":"Science and Technology Facilities Council","keywords":"Protein filament; Outflow; Magnetic field; James Clerk Maxwell Telescope; Field strength; Ejecta; Bipolar outflow; Magnetic energy","score_opus":0.016257655232329596,"score_gpt":0.26586135531875615,"score_spread":0.24960370008642657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2736479339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99835926,0.00005692467,0.00012461684,0.000026230098,0.0000022435481,0.0000056107883,0.0005251824,0.000025201241,0.00087462814],"genre_scores_gemma":[0.99862206,0.000037493992,0.00041828485,0.000018757322,0.000014171644,0.000006669327,0.00073806255,0.000011140257,0.00013333885],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997631,0.000021447197,0.000013792208,0.00007445602,0.00008347765,0.000043735257],"domain_scores_gemma":[0.9987722,0.00009556907,0.00053455343,0.00015924875,0.00016362194,0.00027479528],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002808644,0.00018152848,0.0002167589,0.0018891924,0.00040168833,0.00061073113,0.00033648525,0.00025257148,0.00077590987],"category_scores_gemma":[0.0010043096,0.0001311558,0.00014669233,0.00095364754,0.00028112534,0.0002986618,0.00075546827,0.00019401437,0.00015332946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000111452246,0.000030909854,0.961203,0.000023916466,0.0000583079,0.00017455002,0.0003313289,0.00035617166,0.028041918,0.00015014468,0.00046295303,0.009055355],"study_design_scores_gemma":[0.000004983913,0.000011089229,0.9983955,0.0000029660966,0.0000068809295,0.00004480678,0.000040158793,0.00039922103,0.0005062131,0.000017887442,0.0005673085,0.0000030115218],"about_ca_topic_score_codex":0.012866073,"about_ca_topic_score_gemma":0.023211574,"teacher_disagreement_score":0.012866073,"about_ca_system_score_codex":0.0005321157,"about_ca_system_score_gemma":0.00024398284,"threshold_uncertainty_score":0.025582373},"labels":[],"label_agreement":null},{"id":"W2736568436","doi":"10.3847/1538-4357/aa7fbf","title":"Gas Content and Kinematics in Clumpy, Turbulent Star-forming Disks","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council","keywords":"Astrophysics; Physics; Galaxy; Star formation; Mass fraction; Plateau de Bure Interferometer; Mass ratio; Luminosity; Sigma; Astronomy; Thermodynamics","score_opus":0.021439159804666697,"score_gpt":0.24098731977746604,"score_spread":0.21954815997279933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2736568436","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998431,0.000032344607,0.000025120364,0.0000011040738,1.394123e-7,7.877483e-7,0.00005171395,0.0000018087851,0.00004388257],"genre_scores_gemma":[0.9998154,0.000016231133,0.000033795437,7.003518e-7,5.916521e-7,7.6527294e-7,0.000104632345,6.2637815e-7,0.000027234655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999182,0.0000100039815,0.000008350481,0.000022536908,0.0000138695905,0.000027032967],"domain_scores_gemma":[0.9994735,0.00007799853,0.00024935236,0.000035915557,0.000049931336,0.00011333274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001732586,0.00019849169,0.00018126905,0.0018046817,0.0002876848,0.0006394939,0.00019344637,0.00013578194,0.0006846916],"category_scores_gemma":[0.0007009489,0.00011589824,0.00010895009,0.00066278805,0.0004076522,0.00027305805,0.00035923475,0.00008306204,0.00021361609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009468328,0.00001936274,0.9923424,0.0000064182923,0.000016396094,0.00007350869,0.00022128943,0.00028637963,0.005698031,0.00006520973,0.000018045957,0.0011582316],"study_design_scores_gemma":[0.0000027393169,0.000026918618,0.99838805,0.0000017212403,0.000006388338,0.00012735072,0.00014920635,0.00048408852,0.0007116183,0.00004263645,0.000057197696,0.0000019329404],"about_ca_topic_score_codex":0.004257105,"about_ca_topic_score_gemma":0.0040632854,"teacher_disagreement_score":0.004257105,"about_ca_system_score_codex":0.00027282565,"about_ca_system_score_gemma":0.00008962369,"threshold_uncertainty_score":0.008464694},"labels":[],"label_agreement":null},{"id":"W2736684204","doi":"10.3847/1538-4357/aa8136","title":"Observable Emission Features of Black Hole GRMHD Jets on Event Horizon Scales","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Science and Technology Facilities Council","keywords":"Event horizon; Adiabatic process; Radiative transfer; Black hole (networking); Supermassive black hole; Observable; Magnetohydrodynamics; Jet (fluid)","score_opus":0.014628240437217142,"score_gpt":0.25651855862358125,"score_spread":0.2418903181863641,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2736684204","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949663,0.00014859872,0.0026098324,0.00005976926,0.0000062105964,0.000008174924,0.00017692015,0.00021852889,0.0018056812],"genre_scores_gemma":[0.99932325,0.00001566873,0.00047121313,0.000006579167,0.0000066607463,0.0000026594814,0.000088837136,0.00001265132,0.00007252613],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995744,0.0000060601874,0.0000014497946,0.000011344943,0.000008674347,0.000015029922],"domain_scores_gemma":[0.9996488,0.00007835504,0.00012873205,0.000030591273,0.00002455531,0.00008900611],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015204302,0.00023632702,0.00018078092,0.0003593351,0.00016610768,0.00042971098,0.00025999747,0.0002088333,0.0010802036],"category_scores_gemma":[0.0005122491,0.00011948595,0.0002118082,0.0002017707,0.0003275309,0.0002434918,0.00037305712,0.00036681347,0.00010727568],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019434183,0.00031587822,0.29181555,0.00018969974,0.00023233124,0.0076914397,0.0009902155,0.017838772,0.62806755,0.016118221,0.002129942,0.032666918],"study_design_scores_gemma":[0.00007497483,0.0002447828,0.93374467,0.000021651394,0.000054037275,0.00079250894,0.000119862234,0.039645683,0.01866767,0.00521302,0.0013859014,0.000035229285],"about_ca_topic_score_codex":0.00042304007,"about_ca_topic_score_gemma":0.00026619222,"teacher_disagreement_score":0.0010802036,"about_ca_system_score_codex":0.00024204144,"about_ca_system_score_gemma":0.000040360694,"threshold_uncertainty_score":0.0036136508},"labels":[],"label_agreement":null},{"id":"W2736729055","doi":"10.3847/1538-4357/aaa1ed","title":"Elucidating ΛCDM: Impact of Baryon Acoustic Oscillation Measurements on the Hubble Constant Discrepancy","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":232,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Cosmic microwave background; Hubble's law; Cosmic distance ladder; Galaxy; Cosmology; Baryon acoustic oscillations; Baryon; Oscillation (cell signaling); South Pole Telescope","score_opus":0.023164105232175342,"score_gpt":0.293154462341258,"score_spread":0.2699903571090827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2736729055","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9908324,0.00033178355,0.0039076214,0.00056526414,0.00002416989,0.0000047787353,0.00037508478,0.00005330305,0.0039056304],"genre_scores_gemma":[0.999116,0.000033637916,0.0006232465,0.000027017693,0.00001444492,0.0000014670386,0.000096531316,0.000013876357,0.00007379668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99882394,0.0005969075,0.000040852396,0.00024123969,0.00022256514,0.000074568976],"domain_scores_gemma":[0.98455936,0.011265937,0.001671613,0.0013049542,0.0006748831,0.00052330527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005184789,0.00026230986,0.0003335585,0.0011644701,0.00042765285,0.0013826526,0.0006373142,0.0003753094,0.0013463758],"category_scores_gemma":[0.019597454,0.0001651599,0.00020442758,0.0011542619,0.00072794216,0.00094556995,0.0008620683,0.0005746153,0.00022393311],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038054874,0.00005685139,0.952268,0.000043532436,0.00021002954,0.00031625567,0.0003455887,0.011695514,0.002562068,0.0111492835,0.0012651251,0.019707173],"study_design_scores_gemma":[0.000045409837,0.000082482715,0.8806027,0.00006303732,0.00013631313,0.00015961246,0.0006677797,0.0946407,0.0039371382,0.016355017,0.0032608176,0.000049090562],"about_ca_topic_score_codex":0.004598519,"about_ca_topic_score_gemma":0.0035815446,"teacher_disagreement_score":0.005184789,"about_ca_system_score_codex":0.00061584916,"about_ca_system_score_gemma":0.0003278111,"threshold_uncertainty_score":0.027420104},"labels":[],"label_agreement":null},{"id":"W2736749549","doi":"10.3847/1538-4357/aa9567","title":"Phase Offsets and the Energy Budgets of Hot Jupiters","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"","keywords":"Hot Jupiter; Albedo (alchemy); Planet; Energy budget; Phase (matter); Brightness; Eclipse; Phase lag; Brightness temperature","score_opus":0.01124427214544474,"score_gpt":0.24640041322621212,"score_spread":0.23515614108076738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2736749549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99770087,0.00017152447,0.00030920107,0.0000149372845,0.0000019976776,0.0000025543475,0.0008845792,0.00001878477,0.00089561637],"genre_scores_gemma":[0.9977719,0.00007766283,0.0003582712,0.000006809551,0.000005373606,0.000004812921,0.0016162299,0.000020411526,0.00013853653],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998863,0.000014863709,0.000008630788,0.000043562308,0.000024443325,0.00002228674],"domain_scores_gemma":[0.9995091,0.00010461664,0.00020073,0.00006403583,0.000082096776,0.000039350925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019426241,0.00021584753,0.00017665785,0.0016109754,0.00030516615,0.0005589597,0.000192385,0.0001986231,0.0010815462],"category_scores_gemma":[0.0010877044,0.00019997724,0.00016112307,0.0014796124,0.00027267667,0.00056246057,0.00045920414,0.00017565394,0.00017576234],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073495903,0.00004350553,0.8894041,0.0001569826,0.00021267474,0.00016645071,0.000559707,0.006964285,0.07437349,0.0010989971,0.0006084753,0.025676247],"study_design_scores_gemma":[0.000008305853,0.000047961905,0.9914444,0.000009491636,0.0000268593,0.000066919936,0.0000897739,0.001638064,0.0046445886,0.0003100582,0.0017052285,0.00000835797],"about_ca_topic_score_codex":0.00238455,"about_ca_topic_score_gemma":0.0041082883,"teacher_disagreement_score":0.00238455,"about_ca_system_score_codex":0.00036026945,"about_ca_system_score_gemma":0.0000742231,"threshold_uncertainty_score":0.004741311},"labels":[],"label_agreement":null},{"id":"W2737146793","doi":"10.3847/1538-4357/aa960b","title":"SN 1986J VLBI. IV. The Nature of the Central Component","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Very-long-baseline interferometry; Spectral energy distribution; Spectral index; Nebula; Interferometry; Spectral line; Component (thermodynamics); Shock wave","score_opus":0.008886042863458612,"score_gpt":0.2332691924935052,"score_spread":0.22438314963004657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2737146793","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948967,0.00026209408,0.0012208808,0.000028513643,0.000008556899,0.000011371391,0.0011296831,0.000084481835,0.0023577942],"genre_scores_gemma":[0.99543434,0.000059476206,0.0012294973,0.000023183295,0.000007505383,0.000005220912,0.0022522658,0.000019165393,0.0009694083],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989283,0.000007233975,0.0000044772737,0.000035852376,0.000030467038,0.000029044748],"domain_scores_gemma":[0.9996958,0.000020664344,0.00013160767,0.000028082044,0.00006668496,0.0000572237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024539264,0.00023162634,0.00026457995,0.00064823916,0.00031188322,0.00038396215,0.0002167936,0.0001827147,0.001161703],"category_scores_gemma":[0.0003895444,0.0001831789,0.00016574979,0.00045773853,0.00016651141,0.00013761225,0.00028876716,0.00017506204,0.00053152133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007898116,0.00007374473,0.72829527,0.00009268594,0.00009173699,0.00041203966,0.00012208598,0.0009810167,0.24729154,0.00048955873,0.00085141696,0.020509105],"study_design_scores_gemma":[0.0000041121457,0.00002926558,0.99218386,0.000003708656,0.000012895394,0.000285198,0.000017285063,0.0008318171,0.0055934167,0.0000526184,0.0009821897,0.0000036728466],"about_ca_topic_score_codex":0.0063649365,"about_ca_topic_score_gemma":0.010695654,"teacher_disagreement_score":0.0063649365,"about_ca_system_score_codex":0.0004055711,"about_ca_system_score_gemma":0.000117784344,"threshold_uncertainty_score":0.012655795},"labels":[],"label_agreement":null},{"id":"W2738320264","doi":"10.3847/1538-4357/aa98d9","title":"On the Possibility of Fast Radio Bursts from Inside Supernovae: The Case of SN 1986J","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Ejecta; Supernova; Physics; Astrophysics; Stars; Neutron star; Astronomy","score_opus":0.017414815984360798,"score_gpt":0.25337172857969453,"score_spread":0.23595691259533375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2738320264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.969858,0.0018714673,0.0045930957,0.0019380866,0.000054561006,0.00001615508,0.000065430264,0.000038106577,0.02156516],"genre_scores_gemma":[0.99606675,0.0009003591,0.0009841606,0.00025066294,0.00013884755,0.000004840597,0.000059532045,0.000011757026,0.0015831292],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99978167,0.000058452704,0.000015996944,0.000030004516,0.000034546152,0.00007930176],"domain_scores_gemma":[0.9981542,0.00090883084,0.0004967446,0.00018123737,0.00007383407,0.00018497066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009609533,0.00034165947,0.00031876416,0.0011308495,0.001021221,0.0018021323,0.00038290612,0.0018183464,0.0025737898],"category_scores_gemma":[0.0024424733,0.00025113768,0.000345727,0.000686699,0.0011989133,0.00077942136,0.00090085383,0.0008464108,0.0005536315],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074454525,0.00025049303,0.6534234,0.00012645395,0.00012721006,0.23230226,0.0021732443,0.004075875,0.011184545,0.049624115,0.003105062,0.04286277],"study_design_scores_gemma":[0.00019260721,0.0007147962,0.48616394,0.00032023733,0.00031362943,0.3662199,0.004798329,0.03333047,0.010631233,0.05820869,0.038922463,0.00018364831],"about_ca_topic_score_codex":0.002515491,"about_ca_topic_score_gemma":0.0020850683,"teacher_disagreement_score":0.0025737898,"about_ca_system_score_codex":0.00039862594,"about_ca_system_score_gemma":0.00014843186,"threshold_uncertainty_score":0.008610189},"labels":[],"label_agreement":null},{"id":"W2739709315","doi":"10.3847/1538-4357/aa9ff4","title":"Measurements of the Temperature and E-mode Polarization of the CMB from 500 Square Degrees of SPTpol Data","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":186,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; Canadian Institute for Advanced Research","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of Colorado Boulder; Office of Science; Canada Research Chairs; High Energy Physics; University of Chicago; McGill University; Gordon and Betty Moore Foundation; Argonne National Laboratory; U.S. Department of Energy; National Science Foundation","keywords":"Cosmic microwave background; Polarization (electrochemistry); Multipole expansion; Spectral line; Spectral density; Cosmic background radiation; Flux (metallurgy); Microwave; Sigma","score_opus":0.0213765373021225,"score_gpt":0.27175689227370337,"score_spread":0.25038035497158084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2739709315","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913687,0.000046003042,0.00215766,0.000033674427,0.000007155744,0.000011091619,0.0042478116,0.00012395912,0.0020038506],"genre_scores_gemma":[0.98735154,0.00005849428,0.0023869218,0.000032463708,0.00002041611,0.000032110103,0.009763101,0.00006772887,0.0002873037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996822,0.0000361706,0.000016444092,0.00008589088,0.00011913935,0.000060155035],"domain_scores_gemma":[0.99933136,0.00012585423,0.00016249312,0.00015921913,0.00013589127,0.00008516008],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033343674,0.00043223533,0.00019997188,0.0013305214,0.00027745712,0.00044369805,0.000318342,0.00028577232,0.0015315695],"category_scores_gemma":[0.00075189583,0.00024212869,0.00032468216,0.0016575679,0.0002253871,0.00039281015,0.00048790762,0.00039820434,0.00059764576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005647038,0.0001174874,0.8236433,0.00011275865,0.0002731833,0.00054591586,0.00071791216,0.0047918907,0.12447576,0.0003324105,0.002654433,0.041770153],"study_design_scores_gemma":[0.000011372916,0.00003969023,0.9881684,0.000006801961,0.000031659085,0.00017332245,0.00009228449,0.002284915,0.0070060063,0.00007243174,0.0021011634,0.000011993008],"about_ca_topic_score_codex":0.0030267409,"about_ca_topic_score_gemma":0.0060268794,"teacher_disagreement_score":0.0030267409,"about_ca_system_score_codex":0.00022842194,"about_ca_system_score_gemma":0.0001234838,"threshold_uncertainty_score":0.006018281},"labels":[],"label_agreement":null},{"id":"W2739899950","doi":"10.3847/1538-4357/aa7e7f","title":"Searching for High-energy, Horizon-scale Emissions from Galactic Black Hole Transients during Quiescence","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Magnetosphere; Accretion (finance); Pulsar; Radiative transfer; Photon; Electron; Black hole (networking); Active galactic nucleus; Magnetic field; Eddington luminosity","score_opus":0.016015759814064223,"score_gpt":0.2536954045310133,"score_spread":0.23767964471694908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2739899950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990202,0.000051062725,0.0002623414,0.0000066484786,9.1140936e-7,0.0000025406368,0.00007829665,0.00001293624,0.0005649453],"genre_scores_gemma":[0.99942505,0.00002643902,0.00023174119,0.000005823995,0.0000026499058,0.0000014873631,0.0001711435,0.0000020996795,0.00013353798],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995303,0.0000058060477,0.0000027232,0.000012110022,0.000012604876,0.000013703358],"domain_scores_gemma":[0.99976796,0.000038829716,0.000099443605,0.000020885123,0.000026213156,0.00004671922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022830284,0.00014876938,0.000119397235,0.00092500314,0.0002645257,0.0003548304,0.00018317436,0.00019930737,0.0006986457],"category_scores_gemma":[0.00035920853,0.0000708478,0.00012097024,0.00036170677,0.00010174222,0.0002278881,0.00022777972,0.000086138374,0.00015916029],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024102302,0.000050780905,0.930242,0.00002601922,0.00003393368,0.0003257793,0.00028632922,0.00047536578,0.04905656,0.00030742234,0.00016053497,0.018794198],"study_design_scores_gemma":[0.0000057311363,0.00012289545,0.98893297,0.000008148672,0.00002394336,0.0002993421,0.0001666754,0.0021084507,0.0074753254,0.0001433897,0.000709048,0.000004086572],"about_ca_topic_score_codex":0.0013592481,"about_ca_topic_score_gemma":0.0022173189,"teacher_disagreement_score":0.0013592481,"about_ca_system_score_codex":0.00017720278,"about_ca_system_score_gemma":0.000071352304,"threshold_uncertainty_score":0.0027026534},"labels":[],"label_agreement":null},{"id":"W2740217938","doi":"10.3847/1538-4357/aa951b","title":"Search for an Excess of Events in the Super-Kamiokande Detector in the Directions of the Astrophysical Neutrinos Reported by the IceCube Collaboration","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Regina; University of British Columbia; TRIUMF; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Super-Kamiokande; Physics; Multiplet; Neutrino; Event (particle physics); Detector; Particle physics; Astrophysics; Nuclear physics; Astronomy; Solar neutrino; Neutrino oscillation; Optics","score_opus":0.02413471154527012,"score_gpt":0.29684412653379644,"score_spread":0.2727094149885263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2740217938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99671006,0.00011471666,0.00068537396,0.000022171667,0.000007700959,0.000011073381,0.0010485277,0.000039426744,0.0013609189],"genre_scores_gemma":[0.9935482,0.00010393811,0.0016080772,0.000025406545,0.000017434242,0.000013034714,0.0041573937,0.00003232642,0.000494231],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992793,0.00013836777,0.00005271106,0.00019715451,0.00020690603,0.00012556835],"domain_scores_gemma":[0.997943,0.00060213305,0.00071128854,0.000231632,0.0003027682,0.00020924032],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013735932,0.0003414843,0.00046765315,0.0017144808,0.00035677856,0.0011249261,0.0003148432,0.00027611761,0.0017102129],"category_scores_gemma":[0.0014891755,0.0002084754,0.0005798214,0.0016176623,0.00026024177,0.0004040901,0.00075948384,0.00033478567,0.0003533562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015488468,0.00008072617,0.9621221,0.000074071715,0.00040003363,0.0006120047,0.0001512763,0.0014952848,0.024823546,0.0005189689,0.0007199554,0.0074531985],"study_design_scores_gemma":[0.00005462277,0.00029897445,0.9680232,0.00003224542,0.00028665605,0.0009945602,0.00030468463,0.004676942,0.020674385,0.00036250995,0.0042642886,0.00002695609],"about_ca_topic_score_codex":0.0023224775,"about_ca_topic_score_gemma":0.0041305516,"teacher_disagreement_score":0.0023224775,"about_ca_system_score_codex":0.00039094602,"about_ca_system_score_gemma":0.00042452125,"threshold_uncertainty_score":0.007264316},"labels":[],"label_agreement":null},{"id":"W2740234984","doi":"10.3847/1538-4357/aa835e","title":"Ω-slow Solutions and Be Star Disks","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Polar; Stars; Line (geometry); Rotation (mathematics); Angular velocity; Polar wind; Oblate spheroid","score_opus":0.026356698416903357,"score_gpt":0.26903873922834826,"score_spread":0.2426820408114449,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2740234984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9745126,0.0002107536,0.015147403,0.0003809531,0.00004813942,0.000023745644,0.000081218815,0.00007858062,0.0095167775],"genre_scores_gemma":[0.99559516,0.00008686591,0.002499201,0.000033267574,0.000012654504,0.000012209148,0.000053886757,0.00002118887,0.0016854275],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999285,0.00002167185,0.0000044019007,0.000012127649,0.000012349191,0.00002085993],"domain_scores_gemma":[0.9995639,0.00011810041,0.00012492317,0.00003349364,0.00007061816,0.00008896291],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020992152,0.00049383065,0.0003406105,0.00042149815,0.0004380556,0.00096241565,0.00037737231,0.0007505367,0.0026859078],"category_scores_gemma":[0.0020201816,0.00020105726,0.00031309575,0.00015634538,0.00043930972,0.0005759279,0.00080837356,0.00052493496,0.00026337238],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030211205,0.00020977882,0.035993237,0.00015425634,0.00008035944,0.0016692535,0.0003836512,0.84652174,0.021341518,0.0824707,0.0014270415,0.009446306],"study_design_scores_gemma":[0.0000673559,0.00008007296,0.0037916321,0.000014909756,0.00001014183,0.00015638358,0.00028744695,0.9780862,0.0013761027,0.014376289,0.0017370561,0.000016402422],"about_ca_topic_score_codex":0.0032575857,"about_ca_topic_score_gemma":0.0015130515,"teacher_disagreement_score":0.0032575857,"about_ca_system_score_codex":0.00028216612,"about_ca_system_score_gemma":0.00027599419,"threshold_uncertainty_score":0.008985221},"labels":[],"label_agreement":null},{"id":"W2740973235","doi":"10.3847/1538-4357/aa83ae","title":"An Optically Faint Quasar Survey at z ∼ 5 in the CFHTLS Wide Field: Estimates of the Black Hole Masses and Eddington Ratios","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Quasar; Physics; Astrophysics; Galaxy; Astronomy; Black hole (networking); Accretion (finance); Emission spectrum; Supermassive black hole; Spectral line","score_opus":0.012767446038661203,"score_gpt":0.2565519530213996,"score_spread":0.2437845069827384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2740973235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986362,0.00004181739,0.00012894564,0.000020194202,0.0000011669035,0.00000561696,0.00043151504,0.00000893992,0.0007256071],"genre_scores_gemma":[0.9987484,0.000020624648,0.00014817296,0.00002150014,0.000002894842,0.0000036630581,0.0006693928,0.0000012435751,0.00038404105],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998584,0.0000146842485,0.000006327222,0.000032346707,0.000037845595,0.00005038104],"domain_scores_gemma":[0.9993074,0.000051603347,0.00016155378,0.000047579146,0.00014707493,0.0002847155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004124612,0.00017067006,0.000118112985,0.0020032628,0.00045486083,0.00035345342,0.00020260875,0.00013887613,0.0017474947],"category_scores_gemma":[0.0004051603,0.00008925524,0.0001452685,0.00057118584,0.00024168816,0.0002145698,0.00035473518,0.00013672728,0.00024750715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000020991065,0.00001311343,0.99397874,0.0000031479374,0.000010461101,0.000048483827,0.00016999933,0.000043970274,0.0030820929,0.00004525913,0.00016197072,0.0024217106],"study_design_scores_gemma":[7.739379e-7,0.0000108505155,0.9994407,0.0000012016217,0.0000027655742,0.000018245986,0.00009613249,0.000058717553,0.00015743678,0.000005481501,0.00020643207,0.0000011789997],"about_ca_topic_score_codex":0.12093585,"about_ca_topic_score_gemma":0.22180964,"teacher_disagreement_score":0.12093585,"about_ca_system_score_codex":0.0005870865,"about_ca_system_score_gemma":0.00029630438,"threshold_uncertainty_score":0.24046385},"labels":[],"label_agreement":null},{"id":"W2741530808","doi":"10.3847/1538-4357/aa7beb","title":"Adding the s-Process Element Cerium to the APOGEE Survey: Identification and Characterization of Ce ii Lines in the H-band Spectral Window","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Magyar Tudományos Akadémia; Ministerio de Economía y Competitividad; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; National Research, Development and Innovation Office; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Milky Way; Stars; Giant star; Asymptotic giant branch; s-process; Red giant; Red clump; Astronomy; Open cluster; Spectral line; Abundance of the chemical elements; Red-giant branch; Nucleosynthesis; Metallicity","score_opus":0.017656189054466354,"score_gpt":0.26166148294307967,"score_spread":0.2440052938886133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2741530808","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993771,0.000024612444,0.00013498981,0.000005920014,7.750519e-7,0.0000019210345,0.00012891399,0.000005557118,0.00032024647],"genre_scores_gemma":[0.9988341,0.000029918043,0.0004601674,0.000017190305,0.0000028680877,0.0000035529351,0.00042760395,0.0000039718875,0.00022059205],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998945,0.000011821019,0.0000072612893,0.000043495333,0.000021968533,0.00002097048],"domain_scores_gemma":[0.9996935,0.000044592245,0.00008649603,0.000040485127,0.00007006433,0.00006479946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021266539,0.0001674417,0.00014613585,0.0012086338,0.00020141741,0.0003534945,0.00017233263,0.00020062715,0.00061077275],"category_scores_gemma":[0.0002940533,0.00008633508,0.00011682763,0.00058739487,0.00015471202,0.0002109118,0.0003181263,0.00012335092,0.00017680145],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019117241,0.000041975905,0.9147221,0.00001512606,0.00002878325,0.00011172852,0.00014089316,0.0000916852,0.07795242,0.000057609468,0.00011925855,0.006527315],"study_design_scores_gemma":[0.00000429276,0.000033951423,0.9958354,0.0000015842942,0.00000709745,0.00010932105,0.000091816706,0.00014997451,0.0033391635,0.000010949712,0.00041455915,0.0000019595425],"about_ca_topic_score_codex":0.00219739,"about_ca_topic_score_gemma":0.0047565247,"teacher_disagreement_score":0.00219739,"about_ca_system_score_codex":0.00013119908,"about_ca_system_score_gemma":0.00006077948,"threshold_uncertainty_score":0.0043691993},"labels":[],"label_agreement":null},{"id":"W2742186264","doi":"10.3847/1538-4357/aa7e2b","title":"Robust Cross-correlation-based Measurement of Clump Sizes in Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Galaxy; Redshift; Spiral galaxy; Star formation; Correlation function (quantum field theory); Gaussian; Molecular cloud; Galaxy formation and evolution","score_opus":0.02198418257949027,"score_gpt":0.24065976887675247,"score_spread":0.2186755862972622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2742186264","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9260001,0.00012714214,0.07135605,0.000028385697,0.000010677427,0.000021689932,0.0004516048,0.001006864,0.0009973929],"genre_scores_gemma":[0.9845108,0.000023803446,0.014980831,0.000014262297,0.000010559241,0.000010250317,0.0003277667,0.000034196248,0.000087522945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968183,0.00005653671,0.000013748067,0.00011089532,0.00009431753,0.000042840114],"domain_scores_gemma":[0.9971439,0.0008464864,0.0006459652,0.00048504418,0.0006391749,0.00023949315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00090737495,0.0002894618,0.00031872618,0.002207857,0.00018350493,0.0005022955,0.0005600337,0.0004267362,0.000433653],"category_scores_gemma":[0.004011964,0.0002377665,0.00024742316,0.0008009417,0.00035724742,0.0005329494,0.000677703,0.00027466385,0.0002476946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008798878,0.00029112797,0.41485682,0.00020854111,0.00041721648,0.00038424862,0.00043805133,0.16924939,0.23939157,0.004513772,0.0023049742,0.16706443],"study_design_scores_gemma":[0.000019266676,0.000075077405,0.30556977,0.000018075147,0.00004872482,0.00024563723,0.000044050747,0.65556735,0.03672042,0.001140466,0.00048990507,0.00006121986],"about_ca_topic_score_codex":0.0031072516,"about_ca_topic_score_gemma":0.0035874133,"teacher_disagreement_score":0.0031072516,"about_ca_system_score_codex":0.0006525338,"about_ca_system_score_gemma":0.00025635472,"threshold_uncertainty_score":0.0061783195},"labels":[],"label_agreement":null},{"id":"W2742263520","doi":"10.3847/1538-4357/aa7de2","title":"The Pan-STARRS1 Medium-deep Survey: Star Formation Quenching in Group and Cluster Environments","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Max-Planck-Gesellschaft; Space Telescope Science Institute; National Science Council; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Quenching (fluorescence); Cluster (spacecraft); Star formation; Galaxy; Stars; Galaxy cluster; Stellar mass; Group (periodic table)","score_opus":0.009213072408598366,"score_gpt":0.21659783378157738,"score_spread":0.207384761372979,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2742263520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995978,0.00008827073,0.00049715326,0.00002203166,0.0000023848443,0.0000103349175,0.0026280137,0.00014820253,0.00062561774],"genre_scores_gemma":[0.9896595,0.000039243878,0.0010248958,0.000017010458,0.000008355369,0.000013091945,0.0087923,0.000051154482,0.00039452972],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99952567,0.00010502624,0.000021643566,0.00015699927,0.00010281978,0.000087853026],"domain_scores_gemma":[0.9989447,0.0001068104,0.0003544117,0.00027263994,0.00012731641,0.00019421194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010802565,0.00028506233,0.00040307848,0.0013497575,0.00026239964,0.0004666312,0.0004686487,0.0002174144,0.0011515865],"category_scores_gemma":[0.0014911551,0.00017505119,0.0004730287,0.0009780038,0.00018450955,0.00040270976,0.0009124985,0.0002207347,0.00058334495],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018434902,0.000038678892,0.98023087,0.00004628242,0.0001832395,0.00005945609,0.00018214325,0.0012569373,0.0040833545,0.00013377443,0.0016747091,0.01192613],"study_design_scores_gemma":[0.000009075971,0.00004416736,0.9955415,0.0000039166302,0.000028013475,0.000058491874,0.000077361925,0.0022684338,0.0005972835,0.000041325296,0.001325513,0.000004960878],"about_ca_topic_score_codex":0.007760631,"about_ca_topic_score_gemma":0.009373585,"teacher_disagreement_score":0.007760631,"about_ca_system_score_codex":0.00027732385,"about_ca_system_score_gemma":0.00018429082,"threshold_uncertainty_score":0.015430927},"labels":[],"label_agreement":null},{"id":"W2742803400","doi":"10.3847/1538-4357/aa7f77","title":"A Spectral-line Analysis of the G8 III Standard ε VIR","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Granulation; Radial velocity; Line (geometry); Effective temperature; Luminosity; Flattening; Diagram; Stars; Astronomy; Galaxy; Geometry; Statistics","score_opus":0.01247493610616587,"score_gpt":0.25237951012422216,"score_spread":0.2399045740180563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2742803400","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99881506,0.000016201568,0.00017815533,0.0000045691518,0.0000010029086,0.0000032577457,0.0004158146,0.000021871774,0.00054425007],"genre_scores_gemma":[0.99757403,0.000009865757,0.00032893027,0.0000070562214,0.000001476774,0.0000038374396,0.0017564769,0.000012104206,0.00030628723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999938,0.0000045969464,0.000004544253,0.000020772502,0.000017133172,0.000014870376],"domain_scores_gemma":[0.9996966,0.00002410838,0.00008184082,0.00005320316,0.00008286091,0.000061357416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001281501,0.00012577164,0.00012567932,0.0009255925,0.00022677745,0.00023175027,0.00014957503,0.00012358381,0.0008267215],"category_scores_gemma":[0.00024829496,0.000072415336,0.00019961566,0.0007238936,0.00012112688,0.00008754272,0.00023118529,0.00011472992,0.00034157123],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007356278,0.00010676392,0.8183284,0.00004070311,0.000083929444,0.00030137633,0.00046602995,0.0006815748,0.15060219,0.00026441968,0.00087677664,0.027512271],"study_design_scores_gemma":[0.0000025994343,0.00005728718,0.9965513,0.0000012875571,0.000008813554,0.00011460217,0.00005279752,0.00033345234,0.002278643,0.000024206121,0.0005730349,0.0000019460324],"about_ca_topic_score_codex":0.0039408933,"about_ca_topic_score_gemma":0.0053436034,"teacher_disagreement_score":0.0039408933,"about_ca_system_score_codex":0.00021644519,"about_ca_system_score_gemma":0.00007249749,"threshold_uncertainty_score":0.007835865},"labels":[],"label_agreement":null},{"id":"W2743457834","doi":"10.3847/1538-4357/aa8560","title":"A Widespread, Clumpy Starburst in the Isolated Ongoing Dwarf Galaxy Merger dm1647+21","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Dwarf galaxy; Star formation; Astronomy; Stellar mass; Interstellar medium; Metallicity; Sky","score_opus":0.01077766823990078,"score_gpt":0.2347318167060852,"score_spread":0.22395414846618442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2743457834","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996995,0.000032469816,0.000054534743,0.000007021213,0.000001068799,0.0000012209804,0.00003363863,0.0000038334047,0.00016675047],"genre_scores_gemma":[0.99980253,0.000005652108,0.000057710913,0.000004173824,0.0000017666697,7.5638434e-7,0.00007408362,7.5634756e-7,0.000052503856],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990773,0.000011651165,0.0000067601627,0.000031625998,0.000020700403,0.00002148502],"domain_scores_gemma":[0.99973625,0.000030023473,0.000104354905,0.000014427776,0.000024923445,0.000090023066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012366491,0.00012635198,0.00021447652,0.0005464134,0.00043569412,0.0003657301,0.00018035274,0.00019486589,0.00059261674],"category_scores_gemma":[0.00027834208,0.00008277265,0.000107714404,0.0002189908,0.00019859771,0.00013570415,0.00050136395,0.00015931638,0.000116673655],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026058272,0.000106698135,0.9009821,0.00003352504,0.00008756918,0.0023735233,0.00041048427,0.0005885428,0.08841536,0.0002737979,0.00038448197,0.006083334],"study_design_scores_gemma":[0.0000075813305,0.000091792346,0.99404955,0.0000038518124,0.00002037047,0.0011021345,0.00023907394,0.0013093938,0.0025745607,0.0000827311,0.00051332253,0.0000055511496],"about_ca_topic_score_codex":0.002242243,"about_ca_topic_score_gemma":0.0039535477,"teacher_disagreement_score":0.002242243,"about_ca_system_score_codex":0.00021906263,"about_ca_system_score_gemma":0.000078647005,"threshold_uncertainty_score":0.0044584274},"labels":[],"label_agreement":null},{"id":"W2744175753","doi":"10.3847/1538-4357/aa7b73","title":"Toward an Empirical Theory of Pulsar Emission. XII. Exploring the Physical Conditions in Millisecond Pulsar Emission Regions","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Pulsar; Millisecond pulsar; Astrophysics; Magnetosphere; Binary pulsar; Curvature; Polar; Context (archaeology); Magnetic field; Magnetic dipole; Astronomy; Geometry","score_opus":0.07538952775817269,"score_gpt":0.3837055252440776,"score_spread":0.3083159974859049,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2744175753","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.30805936,0.003209916,0.65695053,0.0073275813,0.00012326552,0.00016394645,0.0008199489,0.0006617062,0.02268369],"genre_scores_gemma":[0.95391583,0.0010977802,0.041869126,0.00022318904,0.00018534387,0.0001828212,0.00047072768,0.00015414551,0.0019009853],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992919,0.00034121174,0.000034989163,0.00017646363,0.00011549437,0.000039793682],"domain_scores_gemma":[0.9887417,0.008033829,0.0014690004,0.0007902712,0.0007457756,0.00021944559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0039499816,0.00056800473,0.0006318453,0.0027876971,0.0008054816,0.0025683737,0.0016547352,0.0010775502,0.0050353417],"category_scores_gemma":[0.021765865,0.0005008056,0.00080361555,0.0019710136,0.004096121,0.0059194025,0.0018055195,0.0020141879,0.00072682375],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006311585,0.00020424003,0.15177491,0.0002689601,0.00026123607,0.00041674502,0.0012044458,0.07505454,0.0017959924,0.70577693,0.003705181,0.059473686],"study_design_scores_gemma":[0.000022641561,0.000051172567,0.056056354,0.00009355874,0.000028755896,0.00041148774,0.0005436621,0.32213712,0.00030607326,0.61676717,0.0035425944,0.000039385926],"about_ca_topic_score_codex":0.0022746464,"about_ca_topic_score_gemma":0.0011210355,"teacher_disagreement_score":0.0050353417,"about_ca_system_score_codex":0.0014448095,"about_ca_system_score_gemma":0.00057629443,"threshold_uncertainty_score":0.020889759},"labels":[],"label_agreement":null},{"id":"W2744236123","doi":"10.3847/1538-4357/aa844f","title":"Individual, Model-independent Masses of the Closest Known Brown Dwarf Binary to the Sun","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Astrometry; Proper motion; Brown dwarf; Barycentric coordinate system; Radial velocity; Orbit (dynamics); Observatory; Sky; Orbital motion","score_opus":0.024710621152576,"score_gpt":0.2587153673137028,"score_spread":0.23400474616112682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2744236123","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99750406,0.000059843238,0.0014016553,0.000035032514,0.00000709675,0.000005397594,0.00032208202,0.000026566522,0.0006382402],"genre_scores_gemma":[0.99885225,0.000010708288,0.00036573684,0.0000055431824,0.0000029911441,0.0000031555078,0.00050991855,0.000007301122,0.00024238415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999788,0.00005874042,0.000007666133,0.00009869156,0.000020071833,0.000026915031],"domain_scores_gemma":[0.99911374,0.0003325218,0.00014836546,0.00019165671,0.00007753282,0.00013607666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00112901,0.00020391984,0.00048073853,0.00042173447,0.0005910855,0.00080083346,0.00060860504,0.00038306712,0.002103429],"category_scores_gemma":[0.0031436426,0.00023044036,0.00043445508,0.00024640805,0.00040289198,0.00048421795,0.00064808904,0.00031460827,0.00045341408],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048126432,0.000094195304,0.70977974,0.000041597814,0.00034309854,0.0002050989,0.0002131725,0.27337953,0.003392972,0.0030034448,0.0015453326,0.007520498],"study_design_scores_gemma":[0.00006497827,0.00011517129,0.34569314,0.000033114935,0.00012555516,0.00022526683,0.00018139667,0.6453062,0.0018902407,0.004722358,0.0015988823,0.000043724685],"about_ca_topic_score_codex":0.011656366,"about_ca_topic_score_gemma":0.012892194,"teacher_disagreement_score":0.011656366,"about_ca_system_score_codex":0.000787866,"about_ca_system_score_gemma":0.00035790174,"threshold_uncertainty_score":0.023177028},"labels":[],"label_agreement":null},{"id":"W2745604495","doi":"10.3847/1538-4357/aa88ab","title":"Dwarf Galaxy Discoveries from the KMTNet Supernova Program. I. The NGC 2784 Galaxy Group<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Dwarf galaxy; Surface brightness; Galaxy; Supernova; Photometry (optics); RADIUS; Population; Luminosity","score_opus":0.011304660947676397,"score_gpt":0.23254467022746034,"score_spread":0.22124000927978393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2745604495","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924482,0.00011988596,0.00018582633,0.000055186658,0.000011398147,0.000010913384,0.0030238903,0.000043205113,0.0041014883],"genre_scores_gemma":[0.9882975,0.000091157686,0.0006118777,0.000020059644,0.00002150227,0.000011394216,0.008762872,0.000023017497,0.002160579],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984694,0.000010877724,0.000011645279,0.00002992674,0.00005880218,0.00004185308],"domain_scores_gemma":[0.99920386,0.000054769705,0.00026179574,0.0000939376,0.00009971151,0.000285981],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002931676,0.0002443609,0.00020957494,0.0015271476,0.0003736276,0.00046764777,0.00030386986,0.00011759311,0.0028387615],"category_scores_gemma":[0.0005421139,0.00008948252,0.00020884525,0.0008138988,0.0002674989,0.00019629771,0.0006952732,0.00014394493,0.0006534362],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043195023,0.000038597347,0.9737637,0.00003052169,0.000045150184,0.0008664488,0.00019226076,0.00022229295,0.009799919,0.00036072542,0.0019659246,0.01228246],"study_design_scores_gemma":[0.000008910281,0.000048875445,0.9914526,0.0000056475546,0.000018961833,0.000706135,0.00015253265,0.00016930648,0.0024895521,0.0000874118,0.004855785,0.000004208333],"about_ca_topic_score_codex":0.00811127,"about_ca_topic_score_gemma":0.01815455,"teacher_disagreement_score":0.00811127,"about_ca_system_score_codex":0.00048975606,"about_ca_system_score_gemma":0.0002479025,"threshold_uncertainty_score":0.016128123},"labels":[],"label_agreement":null},{"id":"W2746321994","doi":"10.3847/1538-4357/aa8631","title":"The Green Bank Ammonia Survey: Dense Cores under Pressure in Orion A","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Victoria; University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Green Bank Telescope; Virial theorem; Molecular cloud; Astrophysics; Thermal; Physics; Velocity dispersion; High pressure; James Clerk Maxwell Telescope; Astronomy; Star formation; Stars; Meteorology; Mechanics; Galaxy","score_opus":0.021229621146450713,"score_gpt":0.2711295411803093,"score_spread":0.24989992003385858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2746321994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983796,0.00008603261,0.00002735523,0.0000317785,0.0000019404763,0.0000024645499,0.00076332,0.000004016802,0.00070360315],"genre_scores_gemma":[0.9984151,0.00013996767,0.00013772344,0.0000428537,0.000009160341,0.000005935674,0.00085064553,0.000004334332,0.0003943212],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998006,0.000034760265,0.000011226396,0.000058014466,0.000050404564,0.00004498235],"domain_scores_gemma":[0.99898905,0.00012596684,0.0003732511,0.00007253154,0.000096849886,0.0003423957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003122057,0.0001697657,0.00019758966,0.0013700807,0.0005722951,0.00057276076,0.00033275524,0.00018718746,0.001067982],"category_scores_gemma":[0.00067059713,0.00013021943,0.00012108161,0.0011782388,0.00043336125,0.0003839751,0.0010186951,0.00017104704,0.00029227536],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007618089,0.000016854845,0.9930369,0.000013600886,0.000043804408,0.00012607472,0.00040710095,0.000074572534,0.0028255577,0.00008059423,0.00046237322,0.0028363827],"study_design_scores_gemma":[0.0000024369374,0.000008055876,0.9991154,0.0000054508255,0.000004752078,0.000025368829,0.00020791737,0.00006817924,0.00011470074,0.000017907903,0.0004278264,0.0000019537208],"about_ca_topic_score_codex":0.0623347,"about_ca_topic_score_gemma":0.12404583,"teacher_disagreement_score":0.0623347,"about_ca_system_score_codex":0.00049445615,"about_ca_system_score_gemma":0.00045035017,"threshold_uncertainty_score":0.123943746},"labels":[],"label_agreement":null},{"id":"W2748447221","doi":"10.3847/1538-4357/aa855c","title":"The Canada–France Imaging Survey: First Results from the u-Band Component","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; Saint Mary's University; University of Victoria; Royal Military College of Canada; University of Toronto; Dalhousie University; Université de Montréal; University of Waterloo; Herzberg Institute of Astrophysics","funders":"Lawrence Berkeley National Laboratory; Leibniz-Gemeinschaft; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Office of Science; Johns Hopkins University; University of Utah; Centre National de la Recherche Scientifique; Carnegie Institution of Washington; Max-Planck-Institut für Astrophysik; U.S. Department of Energy; Eötvös Loránd Tudományegyetem; Smithsonian Institution; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Milky Way; Sky; Galaxy; Surface brightness; Redshift; Metallicity; Population; Dwarf galaxy; Brightness; Local Group","score_opus":0.01273196971046533,"score_gpt":0.2296205930123136,"score_spread":0.21688862330184827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2748447221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9016122,0.0029972447,0.002722003,0.0018434741,0.00005948974,0.00025124179,0.05445163,0.00041401203,0.035648674],"genre_scores_gemma":[0.9345367,0.001173578,0.00706621,0.0005610257,0.000074862735,0.000097970624,0.045009673,0.00012909228,0.0113508245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990615,0.0001090902,0.00002178731,0.00012985335,0.000326403,0.00035132997],"domain_scores_gemma":[0.99793434,0.000084687264,0.00015685939,0.00011235226,0.001324224,0.00038750572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007731064,0.00053272716,0.00031572182,0.0026364543,0.0013009903,0.0011383209,0.0006719672,0.0003852612,0.0020390877],"category_scores_gemma":[0.0012342099,0.00022839951,0.00041913913,0.0035412365,0.00037991352,0.0003686833,0.0010325611,0.00039631934,0.00067979755],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":true,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003501305,0.000157483,0.8863196,0.000106881365,0.0002648305,0.00043731806,0.0010098959,0.001085893,0.0049245018,0.0019269136,0.038215473,0.06520114],"study_design_scores_gemma":[0.000015480407,0.000022846443,0.9797497,0.000021175903,0.000026821259,0.00007839251,0.0003808819,0.000481687,0.00051338266,0.000038138733,0.018653378,0.000018090112],"about_ca_topic_score_codex":0.97793627,"about_ca_topic_score_gemma":0.98565185,"teacher_disagreement_score":0.022063732,"about_ca_system_score_codex":0.008531257,"about_ca_system_score_gemma":0.009355868,"threshold_uncertainty_score":0.061898887},"labels":[],"label_agreement":null},{"id":"W2748766803","doi":"10.1086/344709","title":"The EXPLORE Project. I. A Deep Search for Transiting Extrasolar Planets","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Exoplanet; Planet; Radial velocity; Physics; Transit (satellite); Astronomy; RADIUS; Astrophysics; Stars; Earth radius; Computer science","score_opus":0.031201928212823984,"score_gpt":0.26401447627238234,"score_spread":0.23281254805955837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2748766803","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.39661565,0.021612626,0.14495093,0.020065239,0.0020963731,0.004681731,0.20848054,0.039898753,0.16159824],"genre_scores_gemma":[0.27733633,0.00508479,0.34952587,0.0054769367,0.001092762,0.0025626516,0.2848702,0.0047244816,0.06932598],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.998938,0.00017340943,0.000032340453,0.00026748775,0.00040378352,0.00018488937],"domain_scores_gemma":[0.9978866,0.00025481725,0.00026903878,0.00032292755,0.00025713124,0.0010093999],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027478114,0.0013684612,0.0005562315,0.0017422703,0.00084465207,0.0022721426,0.0012366223,0.0008508461,0.004485607],"category_scores_gemma":[0.0018318213,0.0005218929,0.0005214059,0.0013766892,0.00074973144,0.001990383,0.0061603035,0.0012817382,0.0037229236],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015600332,0.0005016129,0.074659444,0.000838265,0.00027778218,0.000675248,0.0018313144,0.002600488,0.043400306,0.013554003,0.30967212,0.5504294],"study_design_scores_gemma":[0.00067959586,0.0010711041,0.08176668,0.00035570873,0.00011520682,0.0015156236,0.00065372774,0.004724027,0.01788952,0.00833702,0.88279355,0.0000982496],"about_ca_topic_score_codex":0.003347479,"about_ca_topic_score_gemma":0.0061094738,"teacher_disagreement_score":0.004485607,"about_ca_system_score_codex":0.0006693782,"about_ca_system_score_gemma":0.0015841585,"threshold_uncertainty_score":0.015005827},"labels":[],"label_agreement":null},{"id":"W2750046376","doi":"10.3847/1538-4357/aab35c","title":"Multiwavelength Observations of the Blazar BL Lacertae: A New Fast TeV Gamma-Ray Flare","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Office of Science; Max-Planck-Institut für Astronomie; Russian Science Foundation; Ministerio de Economía y Competitividad; Swinburne University of Technology; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Alexander von Humboldt-Stiftung; Russian Foundation for Basic Research; National Aeronautics and Space Administration; U.S. Department of Energy; Instituto de Astrofísica de Andalucía; National Science Foundation","keywords":"Physics; Blazar; Astrophysics; Flare; Superluminal motion; BL Lac object; Gamma ray; Lorentz factor; Quasar; Light curve; Crab Nebula; Flux (metallurgy); Astronomy; Very Long Baseline Array; Galaxy; Lorentz transformation","score_opus":0.01619932956158543,"score_gpt":0.2285467217528899,"score_spread":0.21234739219130447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2750046376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972274,0.00030868963,0.0004820517,0.000067768546,0.000005753765,0.000009757224,0.00029698652,0.00006680295,0.001534854],"genre_scores_gemma":[0.9979766,0.00008887849,0.0009028201,0.000046103884,0.000017531702,0.000004419825,0.0003535216,0.000009211768,0.0006010231],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993706,0.000004476771,0.0000028321208,0.000014858582,0.000022512004,0.000018246988],"domain_scores_gemma":[0.9997801,0.000023796003,0.00008173806,0.000022348095,0.000027324382,0.000064716696],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015169852,0.00017031988,0.0001434838,0.0007691375,0.00025102566,0.00048360677,0.00021103412,0.00028276505,0.0010234904],"category_scores_gemma":[0.00021839883,0.00014061789,0.00024066077,0.00025736395,0.00013251246,0.0002090391,0.00026549646,0.00032856988,0.00016319107],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040865835,0.00013157183,0.51834726,0.00007094608,0.00018764976,0.0015893743,0.0004018516,0.0005639662,0.4404418,0.00035148312,0.00089981477,0.036605585],"study_design_scores_gemma":[0.000008995134,0.00006040294,0.99523455,0.0000047523554,0.00001766467,0.00044038598,0.000028844415,0.00039029302,0.0027626622,0.00004277491,0.0010028101,0.0000058697974],"about_ca_topic_score_codex":0.0034344771,"about_ca_topic_score_gemma":0.009355068,"teacher_disagreement_score":0.0034344771,"about_ca_system_score_codex":0.00034599425,"about_ca_system_score_gemma":0.00007823634,"threshold_uncertainty_score":0.0068289638},"labels":[],"label_agreement":null},{"id":"W2750206884","doi":"10.3847/1538-4357/aa8562","title":"Chemical Mapping of the Milky Way with The Canada–France Imaging Survey: A Non-parametric Metallicity–Distance Decomposition of the Galaxy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; Saint Mary's University; University of Victoria; Royal Military College of Canada; University of Toronto; Dalhousie University; Université de Montréal; University of Waterloo; Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Sky; Metallicity; Stars; Photometry (optics); Galaxy; Halo; Galactic halo; Star count; Local Group","score_opus":0.008158196185811196,"score_gpt":0.21551063675106974,"score_spread":0.20735244056525853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2750206884","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99377394,0.00015352125,0.0018545,0.000057588648,0.0000019928932,0.00001951212,0.0020082654,0.00008264241,0.0020480368],"genre_scores_gemma":[0.99351853,0.00007786161,0.0028352996,0.00001736481,0.0000043732484,0.000012871209,0.0026551276,0.000018291792,0.0008603233],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997775,0.00002115583,0.00000645385,0.000051705178,0.000075305245,0.000067927846],"domain_scores_gemma":[0.99962354,0.000024163422,0.00006479215,0.000032507036,0.00017992432,0.00007505019],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002467059,0.0002937291,0.00019487555,0.0027083778,0.0004748799,0.00078873103,0.00027968705,0.00017938305,0.000928039],"category_scores_gemma":[0.00065709196,0.00011908784,0.00029912626,0.0015914759,0.0002456977,0.00015577515,0.0005136502,0.00014433582,0.00024179352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009702597,0.000027979877,0.94138086,0.000020324234,0.000103064,0.00011536798,0.0002859928,0.005409928,0.013664254,0.00082502206,0.0015803222,0.036489885],"study_design_scores_gemma":[0.000005567519,0.000009317316,0.989949,0.000004136573,0.000009729994,0.000040993844,0.0001412268,0.0069160266,0.00071114546,0.000069812,0.0021354598,0.000007523721],"about_ca_topic_score_codex":0.7225149,"about_ca_topic_score_gemma":0.7133208,"teacher_disagreement_score":0.7225149,"about_ca_system_score_codex":0.0026973472,"about_ca_system_score_gemma":0.0016303121,"threshold_uncertainty_score":0.55823845},"labels":[],"label_agreement":null},{"id":"W2750311801","doi":"10.3847/1538-4357/aa84ae","title":"Where are the Binaries? Results of a Long-term Search for Radial Velocity Binaries in Proto-planetary Nebulae","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Vlaamse regering; Lietuvos Mokslo Taryba; Fonds Wetenschappelijk Onderzoek; Belgian Federal Science Policy Office; Smithsonian Astrophysical Observatory; Fonds De La Recherche Scientifique - FNRS; National Aeronautics and Space Administration; National Science Foundation","keywords":"Radial velocity; Term (time); Astronomy; Physics; Astrophysics; Planetary nebula; Astrobiology; Stars","score_opus":0.024804878026722522,"score_gpt":0.270945016784108,"score_spread":0.24614013875738547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2750311801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992387,0.00019459453,0.00013511162,0.000015060054,0.000001759355,0.0000036006752,0.00015039522,0.0000033666681,0.0002572889],"genre_scores_gemma":[0.9989178,0.00005991914,0.00023714622,0.000019785746,0.00000637083,0.000003629619,0.00049929804,0.0000027309393,0.0002532863],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996147,0.000079576756,0.000030960706,0.00008667739,0.00009782686,0.00009017064],"domain_scores_gemma":[0.9980515,0.0005128232,0.0004921131,0.00016554388,0.00025642998,0.0005216599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009960405,0.00018008758,0.0003390656,0.0010350927,0.000730281,0.00060145603,0.00028021284,0.00034714505,0.00085323385],"category_scores_gemma":[0.0013229746,0.00009632582,0.0002826939,0.0006538299,0.00031282572,0.0004391877,0.0007576997,0.00031779407,0.00034474983],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003312691,0.00015911498,0.9763866,0.000025070249,0.000072483555,0.00041248678,0.0002915624,0.0002838458,0.011211035,0.000054266297,0.0001465425,0.010625754],"study_design_scores_gemma":[0.000002543404,0.00015400801,0.99729,0.0000059124977,0.000029457657,0.00031525415,0.0002006386,0.0003562805,0.0011112768,0.00003510887,0.00049316604,0.0000062954537],"about_ca_topic_score_codex":0.002484586,"about_ca_topic_score_gemma":0.005655225,"teacher_disagreement_score":0.002484586,"about_ca_system_score_codex":0.00022387611,"about_ca_system_score_gemma":0.00019650014,"threshold_uncertainty_score":0.00526762},"labels":[],"label_agreement":null},{"id":"W2750982206","doi":"10.3847/1538-4357/aa8a78","title":"Virgo Redux: The Masses and Stellar Content of Nuclei in Early-type Galaxies from Multiband Photometry and Spectroscopy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Virgo Cluster; Galaxy; Photometry (optics); Stellar population; Spectroscopy; Galaxy cluster; Cluster (spacecraft); Population; Stellar mass","score_opus":0.026371964790221414,"score_gpt":0.2875227418498293,"score_spread":0.2611507770596079,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2750982206","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99179876,0.00027899977,0.0022089155,0.000022983832,0.000002324293,0.000010571316,0.0039619636,0.00027730764,0.0014381824],"genre_scores_gemma":[0.989716,0.00007748679,0.0036129593,0.000014182615,0.0000070578803,0.000013270784,0.0057599554,0.000050167837,0.0007488472],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998528,0.000035824454,0.0000067410447,0.000047221674,0.000038841194,0.00001846524],"domain_scores_gemma":[0.999632,0.00008427841,0.00011434763,0.00006249269,0.000042671945,0.00006417479],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050460524,0.00025256161,0.00018654957,0.0027468852,0.00017693012,0.0005517317,0.00033192828,0.00015882571,0.0014226246],"category_scores_gemma":[0.000846306,0.00015735537,0.00023746406,0.0006912806,0.00017036569,0.00033679497,0.00060000864,0.00011496495,0.0006733721],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022345789,0.000025886698,0.95541656,0.000033747394,0.00010698971,0.00006794846,0.00023063169,0.0033483556,0.0145284515,0.0004120408,0.0015581045,0.024047839],"study_design_scores_gemma":[0.000004226024,0.000015870044,0.9917636,0.000006155025,0.000015843732,0.00008137144,0.000053762265,0.0042494587,0.0024994938,0.00013718192,0.0011652977,0.000007854714],"about_ca_topic_score_codex":0.008285359,"about_ca_topic_score_gemma":0.009094984,"teacher_disagreement_score":0.008285359,"about_ca_system_score_codex":0.00051267014,"about_ca_system_score_gemma":0.000105187966,"threshold_uncertainty_score":0.016474247},"labels":[],"label_agreement":null},{"id":"W2751424203","doi":"10.3847/1538-4357/aa8768","title":"Stellar Dynamics and Star Formation Histories of z ∼ 1 Radio-loud Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Star formation; Stellar mass; Luminous infrared galaxy; Active galactic nucleus; Radio galaxy; Elliptical galaxy; Galaxy formation and evolution; Stellar dynamics","score_opus":0.007376898531703739,"score_gpt":0.2058300114764911,"score_spread":0.19845311294478737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2751424203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997888,0.000021857195,0.000015537564,0.0000037051902,2.2983515e-7,8.85685e-7,0.00007901711,0.0000013545379,0.00008869639],"genre_scores_gemma":[0.9996526,0.0000152382345,0.00001590747,0.000002411814,9.3132627e-7,8.306486e-7,0.00021408446,6.1628805e-7,0.00009739352],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999931,0.000009272075,0.0000034172508,0.000018156923,0.000010030094,0.0000281673],"domain_scores_gemma":[0.999368,0.000083484694,0.0002968683,0.00003101689,0.000051954223,0.00016873397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019387326,0.00012490644,0.00016461167,0.0011173045,0.0001756268,0.00045212833,0.00018231497,0.00018621936,0.0012193461],"category_scores_gemma":[0.00068177254,0.0000897518,0.000120716155,0.00042175155,0.00023166697,0.00021091985,0.00031332867,0.0001450772,0.00037051976],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041957144,0.00001847489,0.9964504,0.0000024325286,0.000007555747,0.000033311902,0.00016435645,0.00007640253,0.0020307559,0.00004432631,0.000024291592,0.0011056908],"study_design_scores_gemma":[8.8304165e-7,0.000015315316,0.9997067,7.062844e-7,0.0000018893439,0.000023370978,0.00004939188,0.00007479598,0.0000778394,0.000010357733,0.00003819458,7.1905964e-7],"about_ca_topic_score_codex":0.0038821858,"about_ca_topic_score_gemma":0.0049493103,"teacher_disagreement_score":0.0038821858,"about_ca_system_score_codex":0.00019975922,"about_ca_system_score_gemma":0.00006321786,"threshold_uncertainty_score":0.0077192187},"labels":[],"label_agreement":null},{"id":"W2751786664","doi":"10.3847/1538-4357/aa826f","title":"Ohmic Dissipation in Mini-Neptunes","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Ohmic contact; Joule heating; Dissipation; Magnetic field; Planet; Thermal","score_opus":0.012448771201829587,"score_gpt":0.24780475903794813,"score_spread":0.23535598783611855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2751786664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921217,0.0008074815,0.0036010835,0.00006705575,0.000018640361,0.000008213057,0.00012584291,0.000054778866,0.0031951836],"genre_scores_gemma":[0.9984524,0.00008079237,0.00023989982,0.000016885973,0.000006416533,0.000004954219,0.000095311145,0.000010704236,0.0010926862],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999474,0.0000059818176,0.0000025031852,0.000015481926,0.000011034106,0.000017567761],"domain_scores_gemma":[0.99985063,0.000031912186,0.00003325166,0.000020981122,0.000027363027,0.00003581775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008876346,0.00024171144,0.00028485642,0.00023326569,0.00031894227,0.0005276084,0.00022577793,0.00024868254,0.0022955202],"category_scores_gemma":[0.00038075433,0.00014234429,0.00017956975,0.0001727497,0.00023937787,0.00033009262,0.0004928163,0.00028208192,0.00038826556],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012046474,0.00010279495,0.09435965,0.00021642975,0.00017346839,0.0025335217,0.0010016422,0.010818072,0.84344053,0.0035518296,0.001124242,0.04147323],"study_design_scores_gemma":[0.00011310883,0.0008525368,0.72024965,0.00006305007,0.000121336256,0.004756769,0.0011330927,0.059291683,0.17477052,0.013621652,0.024961023,0.000065526576],"about_ca_topic_score_codex":0.00048580463,"about_ca_topic_score_gemma":0.00035861813,"teacher_disagreement_score":0.0022955202,"about_ca_system_score_codex":0.00016975468,"about_ca_system_score_gemma":0.000048929403,"threshold_uncertainty_score":0.0076792836},"labels":[],"label_agreement":null},{"id":"W2752139761","doi":"10.3847/1538-4357/aa9333","title":"ALMA Observations of a Quiescent Molecular Cloud in the Large Magellanic Cloud","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Molecular cloud; Galaxy; Line (geometry); Large Magellanic Cloud; Star cluster; Star formation; Virial theorem; Mean kinetic temperature","score_opus":0.02089631243180473,"score_gpt":0.2664617371497162,"score_spread":0.24556542471791148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2752139761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99899274,0.000046776986,0.00014206498,0.000016042537,0.0000018787302,0.0000034209572,0.00020035653,0.000023129602,0.0005736663],"genre_scores_gemma":[0.99917895,0.000011996543,0.00037926465,0.000007827985,0.0000065697222,0.0000019172899,0.00032463885,0.0000025200547,0.000086249835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999112,0.000008239123,0.0000040186615,0.00002519511,0.000025343219,0.000025905201],"domain_scores_gemma":[0.9997844,0.000031082032,0.000045304598,0.000024356883,0.000030622774,0.000084222556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011623246,0.000115709954,0.0001520439,0.000797232,0.0004536575,0.00032855608,0.00026755958,0.00023893756,0.00072224176],"category_scores_gemma":[0.00028552176,0.00008604716,0.0001389229,0.0004697281,0.00014291509,0.00029045617,0.00032963287,0.00018969372,0.00011821079],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068680703,0.00029170848,0.7992372,0.000044634162,0.000114257455,0.0007882621,0.00045248005,0.0030324438,0.17423923,0.00051497,0.0011210256,0.01947706],"study_design_scores_gemma":[0.000024654468,0.00008217608,0.9898489,0.000004173627,0.000019390936,0.00012108638,0.00011587921,0.005372871,0.0032045052,0.00007910607,0.0011210814,0.0000062298222],"about_ca_topic_score_codex":0.0076771635,"about_ca_topic_score_gemma":0.016026327,"teacher_disagreement_score":0.0076771635,"about_ca_system_score_codex":0.00035642774,"about_ca_system_score_gemma":0.000121251906,"threshold_uncertainty_score":0.015264988},"labels":[],"label_agreement":null},{"id":"W2752166700","doi":"10.3847/1538-4357/aa88c5","title":"CARMA Survey toward Infrared-bright Nearby Galaxies (STING). IV. Spatially Resolved <sup>13</sup>CO in Spiral Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galaxy; Spiral galaxy; Star formation; Line (geometry); Luminous infrared galaxy; Elliptical galaxy; Emission spectrum; Limiting","score_opus":0.019416351734955605,"score_gpt":0.2469764466214903,"score_spread":0.2275600948865347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2752166700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99696153,0.00026757835,0.00014569158,0.0000310006,0.0000030787273,0.000012258361,0.001306317,0.000036454163,0.001236126],"genre_scores_gemma":[0.99596477,0.00013779169,0.0008021773,0.00002754638,0.000012825291,0.000013561435,0.0022810404,0.000008038655,0.00075211655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998098,0.00001993007,0.000009335435,0.000058547186,0.000048811664,0.000053549848],"domain_scores_gemma":[0.99903584,0.00006651605,0.0003300018,0.00012048325,0.00020574598,0.0002413827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029400425,0.00024214764,0.00020032532,0.0020101902,0.0003433072,0.00037169343,0.0003706674,0.00024451682,0.002002828],"category_scores_gemma":[0.0007040989,0.00014386712,0.00021671013,0.001330519,0.00022104684,0.00026566078,0.0005797722,0.00018762864,0.00051733037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001541186,0.000047884023,0.96889144,0.000052330306,0.00005536752,0.00016384762,0.00036787154,0.0001459987,0.011362694,0.000117577685,0.0011097752,0.017531209],"study_design_scores_gemma":[0.000003052936,0.00003390534,0.997964,0.0000049926703,0.000019861487,0.00011301339,0.00009452515,0.00019219898,0.0005204899,0.000013729025,0.0010378987,0.0000022846473],"about_ca_topic_score_codex":0.023328211,"about_ca_topic_score_gemma":0.05527482,"teacher_disagreement_score":0.023328211,"about_ca_system_score_codex":0.00043274034,"about_ca_system_score_gemma":0.00025663694,"threshold_uncertainty_score":0.04638487},"labels":[],"label_agreement":null},{"id":"W2752385875","doi":"10.3847/1538-4357/aa8720","title":"Time-dependent Perpendicular Transport of Energetic Particles for Different Turbulence Configurations and Parallel Transport Models","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Statistical Mechanics and Entropy","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Turbulence; Nonlinear system; Magnetic field; Transport theory; Diffusion; Work (physics); Perpendicular; Field (mathematics); Markov process","score_opus":0.016155232532498336,"score_gpt":0.243247913838479,"score_spread":0.22709268130598065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2752385875","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8004103,0.00052206434,0.18540967,0.000750216,0.00012383144,0.000056357465,0.00014002054,0.00014403522,0.012443533],"genre_scores_gemma":[0.988571,0.00023513836,0.007261989,0.000036843863,0.000041542717,0.000028703114,0.00007357428,0.00003427675,0.0037168793],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985087,0.000043390486,0.000010139058,0.000024467556,0.00003643069,0.00003469835],"domain_scores_gemma":[0.999373,0.00020488557,0.00013938086,0.000055974688,0.00011794922,0.00010883009],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000664892,0.00047400748,0.00053367985,0.0008951801,0.0005880483,0.0011157873,0.0006304537,0.00060443307,0.0012815924],"category_scores_gemma":[0.0013369163,0.00025427103,0.00075328536,0.00034548057,0.0012949161,0.0018306596,0.0007753504,0.00070672034,0.00010867605],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021192204,0.00015372554,0.0029130934,0.00007059667,0.000054045195,0.0003850397,0.00010367146,0.49459726,0.020469025,0.4774492,0.0009223159,0.0026700443],"study_design_scores_gemma":[0.000008648833,0.000015894915,0.00024419941,0.000002057764,0.000005605513,0.000026534597,0.000011327714,0.9799054,0.000644504,0.019014752,0.000110973975,0.000010112031],"about_ca_topic_score_codex":0.003914117,"about_ca_topic_score_gemma":0.0019684003,"teacher_disagreement_score":0.003914117,"about_ca_system_score_codex":0.0013837169,"about_ca_system_score_gemma":0.00078933395,"threshold_uncertainty_score":0.010039628},"labels":[],"label_agreement":null},{"id":"W2752616583","doi":"10.3847/1538-4357/aa8ad2","title":"Calibration of Ultraviolet, Mid-infrared, and Radio Star Formation Rate Indicators","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Astrophysics Division; Science and Technology Facilities Council; College of Engineering, Michigan State University; Tata Institute of Fundamental Research; York University; Office of Science; Johns Hopkins University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; University of Arizona; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Infrared; Ultraviolet; Calibration; Remote sensing; Star (game theory); Star formation; Astrophysics; Environmental science; Astronomy; Physics; Optics; Geography; Stars","score_opus":0.0069597491778596,"score_gpt":0.21214486095831522,"score_spread":0.20518511178045562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2752616583","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8981955,0.0007501354,0.07720432,0.0001296585,0.000097961485,0.00014286177,0.0045162137,0.0023020029,0.016661348],"genre_scores_gemma":[0.97025573,0.00014984606,0.025064323,0.000086509404,0.000032071577,0.00007944835,0.0030222735,0.00012658187,0.0011831952],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9977621,0.000557236,0.00014139448,0.00046687914,0.00093669264,0.00013566895],"domain_scores_gemma":[0.99240184,0.0012547161,0.0019185625,0.0022492548,0.0019223234,0.00025340775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027799981,0.0006354044,0.0002761716,0.0029566023,0.00032993592,0.0007135689,0.00086966483,0.00043986348,0.0016206577],"category_scores_gemma":[0.010665052,0.00026449494,0.0003240399,0.0020547514,0.00036531495,0.00067044375,0.0008023603,0.00052838016,0.0015296908],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016914684,0.00010009927,0.9010625,0.000057998575,0.00011618409,0.00003624298,0.00021567466,0.007238376,0.012294252,0.0013076977,0.0025593454,0.07484242],"study_design_scores_gemma":[0.000024664492,0.00016104389,0.9190597,0.000044262455,0.000058966507,0.00021297586,0.00011636742,0.025264572,0.042720187,0.0012174636,0.011063383,0.000056367095],"about_ca_topic_score_codex":0.0025163444,"about_ca_topic_score_gemma":0.0028219149,"teacher_disagreement_score":0.0029566023,"about_ca_system_score_codex":0.0006443758,"about_ca_system_score_gemma":0.00019655618,"threshold_uncertainty_score":0.0147022605},"labels":[],"label_agreement":null},{"id":"W2753087940","doi":"10.3847/1538-4357/aa863a","title":"A Spatially Resolved Study of Cold Dust, Molecular Gas, H ii Regions, and Stars in the z = 2.12 Submillimeter Galaxy ALESS67.1","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; European Southern Observatory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Council; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Stars; Star formation; Submillimeter Array; Astronomy","score_opus":0.01270839544030764,"score_gpt":0.22808163156749994,"score_spread":0.2153732361271923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753087940","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995875,0.00003334909,0.00007175258,0.00000590663,5.6923756e-7,9.479863e-7,0.00006862179,0.0000066357225,0.00022472469],"genre_scores_gemma":[0.99937457,0.000021858414,0.00024547087,0.000008378917,0.0000031427867,0.0000018544422,0.00020743055,0.0000034297698,0.00013388752],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999622,0.000003037925,0.000001483959,0.000012669977,0.0000072726207,0.000013328872],"domain_scores_gemma":[0.99986506,0.000015377474,0.000046668447,0.000018300741,0.000014576994,0.000040016013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008316087,0.00017808884,0.00019151511,0.0006363149,0.00023031604,0.00029283547,0.00015768099,0.00018030561,0.00046070272],"category_scores_gemma":[0.00014654484,0.00016715105,0.00019712184,0.00038872758,0.00014249598,0.00015740895,0.0002410176,0.00014726218,0.00014858863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001317516,0.00006810867,0.82358396,0.00003347549,0.000088057,0.00042679763,0.0006365495,0.001379609,0.16383424,0.00026991422,0.0002636157,0.009283875],"study_design_scores_gemma":[0.0000025087927,0.000024327986,0.9979614,0.000001681815,0.000006719649,0.00008054436,0.00006557447,0.00066019426,0.0009518831,0.00001903511,0.00022394079,0.0000022795746],"about_ca_topic_score_codex":0.005476698,"about_ca_topic_score_gemma":0.010569142,"teacher_disagreement_score":0.005476698,"about_ca_system_score_codex":0.00025838971,"about_ca_system_score_gemma":0.00009833242,"threshold_uncertainty_score":0.01088959},"labels":[],"label_agreement":null},{"id":"W2753091422","doi":"10.3847/1538-4357/aa8a63","title":"Astrophysical Implications of a New Dynamical Mass for the Nearby White Dwarf 40 Eridani B","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Observatory; Low Mass; Orbital elements; Consistency (knowledge bases); Orbital period; Mass fraction; Brown dwarf","score_opus":0.017681880082162656,"score_gpt":0.26333018292764526,"score_spread":0.2456483028454826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753091422","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9937171,0.00020005158,0.0019293764,0.00029667077,0.000023732855,0.0000038984845,0.00010583035,0.000060912167,0.003662551],"genre_scores_gemma":[0.99868196,0.00005727033,0.0007438128,0.000032815587,0.000016469614,0.0000021736128,0.00010021106,0.000017267288,0.00034800638],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998927,0.000011627058,0.000006377814,0.000046688347,0.000026377533,0.000016127045],"domain_scores_gemma":[0.9997167,0.00003393614,0.00010936348,0.00004152205,0.00003629653,0.00006201275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037437514,0.0003275334,0.000228469,0.00041987596,0.0007283252,0.00079414895,0.000668294,0.0005043936,0.0008187208],"category_scores_gemma":[0.0007215205,0.00020875786,0.00037089983,0.0002170269,0.000516384,0.0006712302,0.0007042845,0.00044874763,0.00022742382],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038405118,0.00011599017,0.7789873,0.000105579646,0.00010192379,0.002335343,0.0013297978,0.020206252,0.13449083,0.03786936,0.002086415,0.021987136],"study_design_scores_gemma":[0.00009926159,0.0002734174,0.80272657,0.00006594639,0.00016129919,0.0020528845,0.0010682263,0.12516545,0.02879837,0.019560268,0.019929178,0.000099204524],"about_ca_topic_score_codex":0.005713752,"about_ca_topic_score_gemma":0.0045920867,"teacher_disagreement_score":0.005713752,"about_ca_system_score_codex":0.0011073695,"about_ca_system_score_gemma":0.00021093796,"threshold_uncertainty_score":0.011361003},"labels":[],"label_agreement":null},{"id":"W2753313542","doi":"10.3847/1538-4357/aa8bb6","title":"Measurements of Physical Parameters of White Dwarfs: A Test of the Mass–Radius Relation","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"White dwarf; Parallax; Physics; Photometry (optics); Astrophysics; RADIUS; Brown dwarf; Stars; Astronomy","score_opus":0.028201539368882898,"score_gpt":0.24505665178485447,"score_spread":0.21685511241597158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753313542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99771106,0.00012295412,0.0012931727,0.000008870621,0.0000018211532,0.0000041506632,0.00014544433,0.00002367765,0.00068884075],"genre_scores_gemma":[0.9992859,0.000018736026,0.00048199896,0.0000028679158,0.0000023074504,0.0000020372852,0.00014063803,0.000003884018,0.000061742365],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994185,0.00014224525,0.000056575966,0.00018199693,0.00016015499,0.000040510287],"domain_scores_gemma":[0.9983542,0.0005352281,0.00039422943,0.0003275572,0.00027714766,0.00011170419],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00075991347,0.00022544472,0.00030017417,0.0015951851,0.00040811294,0.00042888068,0.0003972152,0.00028229447,0.00060138747],"category_scores_gemma":[0.0024759856,0.00012093863,0.000177119,0.0007157987,0.00039990328,0.0003853455,0.0004012635,0.00015458286,0.0004532585],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025104568,0.00005827573,0.91693026,0.00002788189,0.00008155485,0.000100075864,0.0002681361,0.0011585065,0.07144338,0.0006334996,0.00009840432,0.008949074],"study_design_scores_gemma":[0.000008176071,0.00012230044,0.9763847,0.0000044392837,0.000024158593,0.00031053086,0.00013958718,0.005138592,0.016999753,0.00028365935,0.0005749201,0.00000924964],"about_ca_topic_score_codex":0.002029087,"about_ca_topic_score_gemma":0.0015523422,"teacher_disagreement_score":0.002029087,"about_ca_system_score_codex":0.00029670776,"about_ca_system_score_gemma":0.00011432738,"threshold_uncertainty_score":0.004034519},"labels":[],"label_agreement":null},{"id":"W2753348067","doi":"10.3847/1538-4357/aa8958","title":"A Model of the Pulsating Extremely Low-mass White Dwarf Precursor WASP 0247–25B","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Photometry (optics); White dwarf; Astrophysics; Physics; Observable; Surface gravity; Orbital period; Asteroseismology; Stars","score_opus":0.024708780919270236,"score_gpt":0.2413387416069008,"score_spread":0.21662996068763057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753348067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.969522,0.0001365788,0.017949564,0.00044778918,0.000021282745,0.000037899226,0.00020290396,0.00007050522,0.011611505],"genre_scores_gemma":[0.99547535,0.0000665469,0.0019154837,0.000023819692,0.000010629181,0.00003180516,0.000094114155,0.00001412451,0.002368058],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999603,0.000009602615,0.0000017997804,0.000010261615,0.000007938096,0.000010107101],"domain_scores_gemma":[0.99989545,0.000023842864,0.000019462057,0.000008975229,0.000012330906,0.000040060608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001300033,0.00027245862,0.00039269804,0.0003168049,0.00063674717,0.00075055927,0.0008640293,0.0006847803,0.0022878174],"category_scores_gemma":[0.00034117486,0.00019456234,0.00044411913,0.00021528415,0.0005745547,0.0003937533,0.0004445494,0.00027111816,0.00031898855],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004912992,0.00022445059,0.0369851,0.0001635901,0.00012842758,0.0029687542,0.00067882426,0.769499,0.039116055,0.13741714,0.002694164,0.009633268],"study_design_scores_gemma":[0.000088511006,0.00009651087,0.005444535,0.000007631868,0.000021939475,0.00023150032,0.000099136705,0.98442185,0.00061259547,0.007894755,0.001066007,0.000015057269],"about_ca_topic_score_codex":0.009424383,"about_ca_topic_score_gemma":0.0033779044,"teacher_disagreement_score":0.009424383,"about_ca_system_score_codex":0.0006043029,"about_ca_system_score_gemma":0.0005165464,"threshold_uncertainty_score":0.018739045},"labels":[],"label_agreement":null},{"id":"W2753604523","doi":"10.3847/1538-4357/aa8b62","title":"How Do Stars Gain Their Mass? A JCMT/SCUBA-2 Transient Survey of Protostars in Nearby Star-forming Regions","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Dalhousie University; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Astrophysics; Physics; Accretion (finance); Amplitude; Stars; Star formation; Low Mass; Flux (metallurgy); Astronomy; Optics","score_opus":0.030142885611502444,"score_gpt":0.26132824598121795,"score_spread":0.23118536036971551,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753604523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99792033,0.000087048524,0.00010871139,0.00011020758,0.0000025733934,0.0000040596437,0.000634111,0.000017325896,0.0011156421],"genre_scores_gemma":[0.9990845,0.00006644897,0.00014301015,0.00003819768,0.000008971432,0.0000025574702,0.00040522442,0.000004857314,0.0002462692],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998443,0.000016855418,0.000012186276,0.000047859034,0.000042016698,0.000036677124],"domain_scores_gemma":[0.9991084,0.00007625463,0.00029324339,0.00008442044,0.00014740226,0.00029025212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021288329,0.00011948163,0.00019680991,0.0013524406,0.00044251684,0.00082428334,0.00024395491,0.00032412424,0.0011480193],"category_scores_gemma":[0.0011244167,0.00009964998,0.00013050981,0.0015222019,0.0002890553,0.000722226,0.00041340594,0.0002330854,0.00042169887],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003669964,0.00001982009,0.9904653,0.000008943913,0.00001984746,0.00005455177,0.00033295955,0.00008561026,0.0029818674,0.00008650994,0.00042836374,0.0054795374],"study_design_scores_gemma":[8.211479e-7,0.000007877148,0.9992386,0.000001943243,0.0000027380238,0.00003796155,0.00015587838,0.00011657596,0.0001133488,0.000033113178,0.00028978323,0.0000013702665],"about_ca_topic_score_codex":0.010134745,"about_ca_topic_score_gemma":0.023681449,"teacher_disagreement_score":0.010134745,"about_ca_system_score_codex":0.0004217049,"about_ca_system_score_gemma":0.00019304559,"threshold_uncertainty_score":0.020151556},"labels":[],"label_agreement":null},{"id":"W2753717147","doi":"10.3847/1538-4357/aa8ad6","title":"Pressure Distortion of the H<sub>2</sub>–He Collision-induced Absorption at the Photosphere of Cool White Dwarf Stars","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Opacity; White dwarf; Photosphere; Absorption (acoustics); Spectral line; Distortion (music); Absorption spectroscopy; Molecular cloud; Stars","score_opus":0.010324336261109256,"score_gpt":0.2313694123387408,"score_spread":0.22104507607763155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753717147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99765897,0.00007253617,0.00094210164,0.000056480614,0.00000541983,0.0000045404945,0.00007094154,0.00007489605,0.0011140058],"genre_scores_gemma":[0.99965703,0.000020313637,0.00014692447,0.000007661254,0.0000015114707,0.0000022922625,0.000044781755,0.000012071757,0.00010735784],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993086,0.000013114297,0.0000025679449,0.000012242232,0.000021109614,0.000020022257],"domain_scores_gemma":[0.9998305,0.000064214226,0.000030710115,0.000015379363,0.00003117713,0.000027971957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000171583,0.00025248385,0.00019194324,0.00023324412,0.00036841416,0.00038746244,0.00043334597,0.0003176974,0.0012945],"category_scores_gemma":[0.00051126425,0.00019579545,0.00026101133,0.00021048471,0.00041336418,0.00029503755,0.00034085786,0.00036573102,0.00013443963],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078714435,0.00045032092,0.0932754,0.00023303973,0.0002777428,0.0010897549,0.00072334305,0.59386957,0.29012454,0.008618525,0.0013985311,0.009152167],"study_design_scores_gemma":[0.0000812161,0.00011435549,0.07521687,0.000008611232,0.000024711775,0.00009321903,0.00017796551,0.8967174,0.02543969,0.0016078482,0.0004948638,0.000023105895],"about_ca_topic_score_codex":0.0067954655,"about_ca_topic_score_gemma":0.0021613191,"teacher_disagreement_score":0.0067954655,"about_ca_system_score_codex":0.00044889416,"about_ca_system_score_gemma":0.0002489646,"threshold_uncertainty_score":0.0135118365},"labels":[],"label_agreement":null},{"id":"W2753881114","doi":"10.3847/1538-4357/aaa198","title":"The Glitches and Rotational History of the Highly Energetic Young Pulsar PSR J0537–6910","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Astrophysics Division; Astrophysics Science Division; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Goddard Space Flight Center; National Aeronautics and Space Administration; Canada Research Chairs; Smithsonian Astrophysical Observatory","keywords":"Glitch; Pulsar; Amplitude; Magnitude (astronomy); Millisecond pulsar; Rotation (mathematics); Ephemeris; Crab Pulsar","score_opus":0.009349961612895053,"score_gpt":0.2667778147279646,"score_spread":0.25742785311506955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2753881114","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991554,0.0000338287,0.00015905844,0.000004488981,0.0000016151565,0.0000029550226,0.00040709935,0.000013905612,0.00022162682],"genre_scores_gemma":[0.998123,0.00003574543,0.00028237546,0.0000035105618,0.000004295737,0.0000034850466,0.0014569594,0.000007598008,0.000083076615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988997,0.000014955276,0.000009970231,0.000023604543,0.000036490324,0.00002497463],"domain_scores_gemma":[0.99947673,0.0000916789,0.00021332478,0.000047208145,0.00008254324,0.00008862102],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002320607,0.00027782295,0.0002448012,0.0015090132,0.00021961056,0.00029883638,0.00017018286,0.00014461672,0.00056319014],"category_scores_gemma":[0.0007577304,0.00010186823,0.0002654147,0.0007904021,0.00017780498,0.00015440489,0.00023447024,0.00018125004,0.00023056299],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002959462,0.000050165945,0.9427077,0.000036145444,0.00010424437,0.00036539527,0.00017150903,0.0027885071,0.041653987,0.0001025602,0.00030838847,0.01141543],"study_design_scores_gemma":[0.000002706283,0.000050626488,0.9965655,0.0000022685192,0.000008390541,0.00012223724,0.00002893874,0.0018772093,0.001123406,0.000013662511,0.00020015164,0.0000047750627],"about_ca_topic_score_codex":0.009294839,"about_ca_topic_score_gemma":0.012926811,"teacher_disagreement_score":0.009294839,"about_ca_system_score_codex":0.00028416823,"about_ca_system_score_gemma":0.00012940321,"threshold_uncertainty_score":0.018481493},"labels":[],"label_agreement":null},{"id":"W2754100461","doi":"10.3847/1538-4357/aa866c","title":"Determining the Halo Mass Scale Where Galaxies Lose Their Gas<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Universität Hamburg; European Southern Observatory; Science and Technology Facilities Council; European Commission; Alexander von Humboldt-Stiftung; Danmarks Grundforskningsfond; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy group; Galaxy cluster; Astronomy; Galaxy; Luminous infrared galaxy; Accretion (finance); Elliptical galaxy; Radio galaxy; Peculiar galaxy; Population","score_opus":0.0097837425201882,"score_gpt":0.21731026976046094,"score_spread":0.20752652724027273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2754100461","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9865649,0.00042490356,0.002079426,0.00032962355,0.000023080102,0.000009949071,0.0033365886,0.00022035319,0.007011207],"genre_scores_gemma":[0.9974349,0.000057151377,0.00071409997,0.00004379341,0.000025093099,0.000004428156,0.0011519579,0.00002460752,0.00054402027],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989533,0.0000168091,0.0000058603446,0.000032166856,0.000025733169,0.000024114437],"domain_scores_gemma":[0.99837697,0.00058154383,0.00048067112,0.000105445775,0.00017558374,0.00027979375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003145822,0.00015139447,0.00014260391,0.000865953,0.00017740548,0.000813396,0.00031356773,0.0002430555,0.0070162127],"category_scores_gemma":[0.0015711063,0.00009501913,0.00016700896,0.00050875527,0.00027639972,0.00035944424,0.00026708527,0.00015066075,0.0013296461],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016062088,0.000017143257,0.9687526,0.000041259354,0.000052146763,0.000072216564,0.00010914894,0.0013487957,0.013304915,0.0009162727,0.002004133,0.013220797],"study_design_scores_gemma":[0.000003370497,0.000018140388,0.99426234,0.0000061611536,0.000012571282,0.000057061156,0.0001324474,0.0020876874,0.002206355,0.00028576655,0.0009225563,0.0000055798346],"about_ca_topic_score_codex":0.0033394264,"about_ca_topic_score_gemma":0.005421333,"teacher_disagreement_score":0.0070162127,"about_ca_system_score_codex":0.00030798052,"about_ca_system_score_gemma":0.00007066527,"threshold_uncertainty_score":0.023471594},"labels":[],"label_agreement":null},{"id":"W2754253541","doi":"10.3847/1538-4357/aa8c0a","title":"The JCMT Transient Survey: Detection of Submillimeter Variability in a Class I Protostar EC 53 in Serpens Main","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Serpens; Accretion (finance); Brightness; Light curve; Luminosity; James Clerk Maxwell Telescope; Submillimeter Array","score_opus":0.014838459820582224,"score_gpt":0.2527795419196928,"score_spread":0.2379410820991106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2754253541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989178,0.000049578113,0.00005944865,0.000008834391,0.000002667489,0.0000044890567,0.0004299111,0.000018446584,0.00050891866],"genre_scores_gemma":[0.999017,0.000042661963,0.0001430593,0.000010944062,0.000006264826,0.000003933266,0.0006424553,0.0000072402636,0.00012639118],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999083,0.0000060107072,0.0000060231077,0.00003322036,0.000020349906,0.00002601381],"domain_scores_gemma":[0.999645,0.000021491014,0.00015649643,0.00003296315,0.00003497023,0.00010916433],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011804059,0.00020902198,0.00017734003,0.0010341317,0.00028907182,0.00038675487,0.00020005999,0.00019919909,0.0006337279],"category_scores_gemma":[0.0002899601,0.00009558038,0.00015250941,0.0005642446,0.000214033,0.00013312936,0.0004605392,0.00013979302,0.00024686847],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016657855,0.00004529795,0.9572547,0.000032817876,0.000040152514,0.00086808245,0.00043863125,0.00016080237,0.032897957,0.00006897279,0.00045452482,0.0075714523],"study_design_scores_gemma":[0.0000017998498,0.000020278652,0.99837226,0.000003745136,0.000005466817,0.0002439248,0.00007475351,0.000101516816,0.00067616854,0.0000070780698,0.0004916562,0.0000013998956],"about_ca_topic_score_codex":0.006104215,"about_ca_topic_score_gemma":0.009515041,"teacher_disagreement_score":0.006104215,"about_ca_system_score_codex":0.00029169803,"about_ca_system_score_gemma":0.00019514163,"threshold_uncertainty_score":0.012137353},"labels":[],"label_agreement":null},{"id":"W2754564407","doi":"10.3847/1538-4357/aa8d6d","title":"Up and Down the Black Hole Radio/X-Ray Correlation: The 2017 Mini-outbursts from Swift J1753.5−0127","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Curtin University of Technology; University of Leicester","keywords":"Swift; Astrophysics; Physics; Black hole (networking); X-ray; Nuclear physics; Computer science; Computer security","score_opus":0.018466311581223555,"score_gpt":0.24604807209985766,"score_spread":0.2275817605186341,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2754564407","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943104,0.0005147886,0.00038304,0.00028704555,0.0000929294,0.000017236272,0.0010875801,0.00011067774,0.0031963103],"genre_scores_gemma":[0.9966012,0.000117181735,0.00027308887,0.00015953853,0.00010044864,0.000014269342,0.0017969819,0.00006912081,0.00086819206],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998572,0.000009093818,0.0000068600025,0.000034328874,0.000045601366,0.000046859852],"domain_scores_gemma":[0.99959046,0.000038193055,0.00011139671,0.000039051374,0.00006612479,0.0001547251],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000396431,0.0002748304,0.00038431078,0.0008456353,0.0005245231,0.0008178833,0.00025584514,0.00028739282,0.0016065363],"category_scores_gemma":[0.0006359236,0.00014136256,0.0002189386,0.00048233086,0.00039145787,0.00029157405,0.0009407552,0.00056926184,0.0005856795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010439631,0.00023893896,0.86526346,0.00017788031,0.00019443208,0.0035549763,0.0032199903,0.00090399536,0.06326231,0.001686584,0.018338377,0.04211515],"study_design_scores_gemma":[0.000010151664,0.000038525148,0.9938692,0.000016137432,0.000019442416,0.0001727694,0.00028661516,0.00035255362,0.0007098071,0.00013211931,0.0043827225,0.000009855512],"about_ca_topic_score_codex":0.0071922354,"about_ca_topic_score_gemma":0.016900305,"teacher_disagreement_score":0.0071922354,"about_ca_system_score_codex":0.0005357412,"about_ca_system_score_gemma":0.00029805533,"threshold_uncertainty_score":0.014300704},"labels":[],"label_agreement":null},{"id":"W2754798475","doi":"10.3847/1538-4357/aa9c42","title":"Galactic-scale Feedback Observed in the 3C 298 Quasar Host Galaxy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Quasar; Galaxy; Star formation; Supermassive black hole; Submillimeter Array; Outflow; Bulge; Astronomy","score_opus":0.01891773989261261,"score_gpt":0.2376695299682237,"score_spread":0.21875179007561107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2754798475","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994466,0.000018712662,0.000030847903,0.0000066375974,9.65837e-7,0.0000011508571,0.00007400959,0.000012560571,0.00040851792],"genre_scores_gemma":[0.9997836,0.000011088963,0.000024915453,0.00000347759,0.0000017783012,8.275005e-7,0.0000994812,0.0000021149694,0.00007273606],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995375,0.0000027369645,0.0000020618713,0.000011201793,0.000013861489,0.000016509219],"domain_scores_gemma":[0.9997042,0.000022704104,0.00010569829,0.000020711988,0.000045086883,0.000101608544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005267126,0.00016433425,0.00018611783,0.00047022002,0.00018259978,0.0003727306,0.0001688011,0.00015842791,0.0014481388],"category_scores_gemma":[0.00028408697,0.00009367575,0.00007667481,0.00021899787,0.00013881881,0.00013355188,0.00023824805,0.0001485736,0.0002935578],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001562208,0.000093318136,0.8395331,0.000015663067,0.0000339558,0.0005162317,0.00021275306,0.00035373913,0.15314683,0.00019436228,0.00039661475,0.0053471783],"study_design_scores_gemma":[0.0000032078133,0.000028625085,0.9983291,0.0000017653097,0.0000055327923,0.00008771105,0.00007066733,0.00040940518,0.00083690794,0.000023348905,0.00020123187,0.0000024060262],"about_ca_topic_score_codex":0.0060569076,"about_ca_topic_score_gemma":0.008978904,"teacher_disagreement_score":0.0060569076,"about_ca_system_score_codex":0.00022372376,"about_ca_system_score_gemma":0.00007144027,"threshold_uncertainty_score":0.012043297},"labels":[],"label_agreement":null},{"id":"W2754840390","doi":"10.3847/1538-4357/aa831f","title":"Detection and Characterization of Extrasolar Planets through Mean-motion Resonances. II. The Effect of the Planet’s Orbital Eccentricity on Debris Disk Structures","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Planet; Exoplanet; Debris disk; Planetary system; Eccentricity (behavior); Orbital eccentricity; Orbit (dynamics); Transit (satellite); Debris","score_opus":0.007267946304887941,"score_gpt":0.2146992166120561,"score_spread":0.20743127030716815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2754840390","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9649971,0.00031051002,0.032757774,0.000072853465,0.000010364162,0.000030018226,0.00027336087,0.00028920424,0.0012588297],"genre_scores_gemma":[0.96234363,0.00005310056,0.03682402,0.000011997448,0.000006443863,0.0000120328095,0.00035176915,0.000027957383,0.00036900214],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998394,0.000022518223,0.000009369917,0.000066117806,0.000034561657,0.000027936801],"domain_scores_gemma":[0.9992162,0.00018200815,0.00024252867,0.00013678831,0.00009414809,0.00012835646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028457548,0.00021484533,0.00023107532,0.0013012431,0.00031351869,0.0003742133,0.0003501911,0.0004877404,0.00068067753],"category_scores_gemma":[0.00090044964,0.00022924143,0.00032905734,0.00051653566,0.00018445327,0.00034306213,0.00054963946,0.00025317568,0.00046176868],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004434006,0.000109247674,0.22459471,0.0001168931,0.000061609964,0.00043985812,0.0004242309,0.007888118,0.6490651,0.0009422168,0.00064332667,0.115271285],"study_design_scores_gemma":[0.000056997567,0.00033105342,0.5691328,0.00002568854,0.000075595395,0.0020817085,0.00034312095,0.26385063,0.15847638,0.0019007908,0.0036486064,0.00007666263],"about_ca_topic_score_codex":0.0007207704,"about_ca_topic_score_gemma":0.0014980221,"teacher_disagreement_score":0.0013012431,"about_ca_system_score_codex":0.00016777667,"about_ca_system_score_gemma":0.00013124639,"threshold_uncertainty_score":0.0022771358},"labels":[],"label_agreement":null},{"id":"W2755245504","doi":"10.3847/1538-4357/aaa1f1","title":"An Extreme Protocluster of Luminous Dusty Starbursts in the Early Universe","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":190,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Universe; Star formation; Core (optical fiber); Luminous infrared galaxy; Red shift","score_opus":0.013623971684849806,"score_gpt":0.22531484420410025,"score_spread":0.21169087251925045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2755245504","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99713314,0.00018158715,0.0012172406,0.000038046877,0.0000116436695,0.000010163405,0.0003360127,0.000051119263,0.0010210655],"genre_scores_gemma":[0.9978795,0.000057504738,0.0011139822,0.00003872537,0.000011689449,0.000003875882,0.000495854,0.0000074564246,0.00039151395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985194,0.000010362033,0.0000066577268,0.000054922428,0.000034874116,0.000041170475],"domain_scores_gemma":[0.9993137,0.00009369972,0.00017905576,0.000113569076,0.000085780484,0.0002141844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020512518,0.00018393112,0.00021396384,0.0006675975,0.0004403279,0.00071750616,0.00030310254,0.000200392,0.0008752904],"category_scores_gemma":[0.0006680033,0.00013276009,0.00016912782,0.00032746408,0.00039896372,0.00017424834,0.0007477874,0.00022588127,0.00026403135],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000391149,0.00004295966,0.89618844,0.000022950831,0.00005831308,0.0029467852,0.0005115014,0.00033045243,0.082420215,0.0008123828,0.00078432955,0.015490534],"study_design_scores_gemma":[0.000014170656,0.00011518811,0.9760715,0.000011752391,0.000032591186,0.005341874,0.00023786,0.0016479375,0.012458,0.0005047285,0.0035453597,0.000019115787],"about_ca_topic_score_codex":0.002892616,"about_ca_topic_score_gemma":0.0036017082,"teacher_disagreement_score":0.002892616,"about_ca_system_score_codex":0.00030335668,"about_ca_system_score_gemma":0.00013248163,"threshold_uncertainty_score":0.00575155},"labels":[],"label_agreement":null},{"id":"W2756804617","doi":"10.3847/1538-4357/aa8950","title":"Simple Analytical Forms of the Perpendicular Diffusion Coefficient for Two-component Turbulence. III. Damping Model of Dynamical Turbulence","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Turbulence; K-omega turbulence model; K-epsilon turbulence model; Diffusion; Component (thermodynamics); Simple (philosophy); Perpendicular; Mechanics; Classical mechanics; Statistical physics; Thermodynamics; Geometry","score_opus":0.012039321010146459,"score_gpt":0.26275498817151366,"score_spread":0.2507156671613672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2756804617","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08492296,0.0023810964,0.86772114,0.0010687731,0.00037453583,0.00014425369,0.0002727073,0.00035803582,0.042756613],"genre_scores_gemma":[0.92404175,0.0017156531,0.048842344,0.00017856574,0.0002028154,0.00013642365,0.00018154249,0.00014083933,0.024560127],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99990976,0.000021711827,0.000007385943,0.000017402623,0.000030312962,0.000013436628],"domain_scores_gemma":[0.99973804,0.00006800269,0.000057565925,0.000030533844,0.00007761072,0.000028269716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032065454,0.00081439613,0.00030344632,0.0006995415,0.00026535423,0.0007924961,0.00064243196,0.00070783996,0.0027791127],"category_scores_gemma":[0.0015401578,0.00018232715,0.00042271634,0.0003374432,0.00073608407,0.0012468867,0.0005065604,0.0007818409,0.00060072215],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003121182,0.00005035015,0.00074904866,0.00021840718,0.0000146966295,0.00046903893,0.00020882738,0.07500324,0.03272609,0.8759285,0.003078034,0.011522502],"study_design_scores_gemma":[0.000013992444,0.000016616836,0.00053712446,0.000029712515,0.000007405869,0.00034562757,0.00006140668,0.8466796,0.0021727395,0.14625476,0.0038499346,0.000031079824],"about_ca_topic_score_codex":0.0015522853,"about_ca_topic_score_gemma":0.0010070135,"teacher_disagreement_score":0.0027791127,"about_ca_system_score_codex":0.00045440017,"about_ca_system_score_gemma":0.0003621695,"threshold_uncertainty_score":0.0092971325},"labels":[],"label_agreement":null},{"id":"W2758131007","doi":"10.3847/1538-4357/aa8e01","title":"Convection and Overshoot in Models of γ Doradus and δ Scuti Stars","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mount Allison University","funders":"","keywords":"Overshoot (microwave communication); Convection; Stars; Observable; Rotation (mathematics); Convection zone; Rotation period; Variation (astronomy)","score_opus":0.017944730565121875,"score_gpt":0.23687781008434164,"score_spread":0.21893307951921975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2758131007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992717,0.00002318275,0.0003513898,0.000017353908,0.0000010081284,0.000002703403,0.000059325546,0.0000182052,0.00025514225],"genre_scores_gemma":[0.9994887,0.0000120779805,0.00028132417,0.0000043394148,0.0000012551575,0.0000030985764,0.00013835295,0.000007654086,0.00006311033],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985814,0.000041220545,0.000014657633,0.000039511426,0.000021102082,0.00002535454],"domain_scores_gemma":[0.99933404,0.00023301868,0.00011989273,0.00013420857,0.0000725294,0.00010635358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006272347,0.00033825907,0.0004255084,0.00069171126,0.00056081126,0.00095239136,0.0007024277,0.00031150316,0.00054574356],"category_scores_gemma":[0.0017546905,0.00024354916,0.0005271158,0.00060721417,0.00046949025,0.00043260594,0.0005579471,0.0002535153,0.00011180128],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040276058,0.000090907946,0.55015665,0.000033380966,0.00020055033,0.00019973303,0.00025574033,0.43627435,0.0064105885,0.0012514235,0.00030090928,0.004423036],"study_design_scores_gemma":[0.00010307955,0.000105649175,0.12493499,0.000010245491,0.000040669358,0.00014788152,0.00017231374,0.8702326,0.0026612,0.0009949552,0.0005735597,0.000022849807],"about_ca_topic_score_codex":0.013873183,"about_ca_topic_score_gemma":0.0070842295,"teacher_disagreement_score":0.013873183,"about_ca_system_score_codex":0.00097230996,"about_ca_system_score_gemma":0.00039209094,"threshold_uncertainty_score":0.02758485},"labels":[],"label_agreement":null},{"id":"W2758172286","doi":"10.3847/1538-4357/aa8fd0","title":"A <sup>13</sup>CO Detection in a Brightest Cluster Galaxy","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Canadian Space Agency; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; National Science Council; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Galaxy; Cluster (spacecraft); Line (geometry); Emission spectrum; Galaxy cluster; Centroid; Spectral line","score_opus":0.010754092075972912,"score_gpt":0.25090670551720223,"score_spread":0.24015261344122932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2758172286","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965396,0.000073151445,0.00016992104,0.00006485225,0.000008611192,0.000006185916,0.00052829005,0.00013041723,0.002479075],"genre_scores_gemma":[0.99776995,0.000014997387,0.0004798397,0.00005350745,0.000018815746,0.000005990187,0.0009601861,0.000017155997,0.00067946955],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986386,0.00001086701,0.000006811812,0.000038645943,0.000035527555,0.000044250784],"domain_scores_gemma":[0.99936646,0.00005434735,0.00016054808,0.0000762001,0.00011114277,0.00023130566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016729248,0.0001662479,0.0002277632,0.0014300321,0.00045533347,0.0007516121,0.0004013268,0.0003937212,0.0028615585],"category_scores_gemma":[0.00034071004,0.00012629248,0.00016158832,0.00045776673,0.00026314674,0.00018327741,0.0004554181,0.00018788286,0.00065593387],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004754373,0.000082525454,0.866238,0.0000396264,0.00006117577,0.0007131627,0.00022721906,0.00033685175,0.11075899,0.000269844,0.002719245,0.018078016],"study_design_scores_gemma":[0.000009906876,0.0000925628,0.9921747,0.0000046888435,0.000021499003,0.00021657343,0.000052212665,0.0005514441,0.004887544,0.000051049148,0.0019291855,0.000008605249],"about_ca_topic_score_codex":0.005429868,"about_ca_topic_score_gemma":0.01348342,"teacher_disagreement_score":0.005429868,"about_ca_system_score_codex":0.0003952817,"about_ca_system_score_gemma":0.00016627517,"threshold_uncertainty_score":0.010796547},"labels":[],"label_agreement":null},{"id":"W2758885493","doi":"10.3847/1538-4357/aabbae","title":"Low Metallicities and Old Ages for Three Ultra-diffuse Galaxies in the Coma Cluster","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Coma Cluster; Galaxy; Stellar population; Spectral line; Coma (optics); Population; Galaxy groups and clusters; Elliptical galaxy","score_opus":0.010352967054978204,"score_gpt":0.22122983396053195,"score_spread":0.21087686690555374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2758885493","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997422,0.000021490543,0.000029802566,0.000005353793,6.078905e-7,9.935222e-7,0.00004629671,0.0000036892109,0.00014943037],"genre_scores_gemma":[0.99975556,0.0000087523,0.000038875583,0.000005316833,0.000001128518,9.917462e-7,0.0001178693,0.0000011086131,0.0000704103],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998067,0.000014239328,0.000009125798,0.00004047728,0.000042182775,0.00008717557],"domain_scores_gemma":[0.99926037,0.00006197149,0.00014245405,0.00007431382,0.00011777351,0.00034305145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021160977,0.00031173308,0.0003170082,0.0014750578,0.0009003059,0.00066399755,0.0003392413,0.00019616094,0.0011338331],"category_scores_gemma":[0.0005904554,0.0001347037,0.00016768009,0.0007764343,0.00066193525,0.00018337446,0.0007651661,0.00024855242,0.00023183622],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012614566,0.000025698853,0.99254066,0.0000043599866,0.000023439048,0.00013832726,0.00046903567,0.00006158729,0.0040170704,0.0000949306,0.000088692635,0.0024100617],"study_design_scores_gemma":[0.0000028016673,0.000028686525,0.99876356,0.0000012612686,0.0000062411164,0.000107498025,0.00041497,0.000110970264,0.0002928918,0.000036483296,0.00023169826,0.0000030159463],"about_ca_topic_score_codex":0.016000489,"about_ca_topic_score_gemma":0.023898771,"teacher_disagreement_score":0.016000489,"about_ca_system_score_codex":0.0006911281,"about_ca_system_score_gemma":0.0001952831,"threshold_uncertainty_score":0.031814694},"labels":[],"label_agreement":null},{"id":"W2759273283","doi":"10.3847/1538-4357/aa901c","title":"Constraining the Dust Opacity Law in Three Small and Isolated Molecular Clouds","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Opacity; Extinction (optical mineralogy); Optical depth; Cosmic dust; Molecular cloud; Silicate; Thermal emission","score_opus":0.020702133035418027,"score_gpt":0.2477618083750632,"score_spread":0.22705967533964516,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2759273283","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992447,0.000028759721,0.00038898655,0.0000059386743,6.856594e-7,0.0000067761084,0.000044066262,0.000013720619,0.00026642604],"genre_scores_gemma":[0.9996785,0.000007908585,0.00020870581,0.0000026696375,0.0000013882878,0.000001965297,0.00007416378,0.0000032345897,0.000021496204],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985504,0.000016429143,0.000007607941,0.000046681114,0.000030460482,0.000043659347],"domain_scores_gemma":[0.9992132,0.00028358446,0.00016457279,0.000080924285,0.00008074321,0.00017685539],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004980882,0.00045944125,0.0003287544,0.00091398123,0.00043118696,0.00075353734,0.0008805299,0.00042695674,0.00070809096],"category_scores_gemma":[0.0011694023,0.00030281197,0.0004802544,0.00038457024,0.00047550857,0.0004087575,0.0006689812,0.00025397594,0.00010476933],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008738036,0.00038301758,0.8418726,0.00007989744,0.00030122948,0.00048553856,0.0003571533,0.088997185,0.05377578,0.0012668465,0.0002660413,0.011340923],"study_design_scores_gemma":[0.00027398043,0.00022771143,0.7026316,0.000026722295,0.00019917662,0.000095318406,0.00035488364,0.28157145,0.013041322,0.0010232108,0.00051929866,0.00003537854],"about_ca_topic_score_codex":0.021574102,"about_ca_topic_score_gemma":0.017687634,"teacher_disagreement_score":0.021574102,"about_ca_system_score_codex":0.0012547068,"about_ca_system_score_gemma":0.0003511141,"threshold_uncertainty_score":0.042897046},"labels":[],"label_agreement":null},{"id":"W2759719452","doi":"10.3847/1538-4357/aaaa1b","title":"Shaken Snow Globes: Kinematic Tracers of the Multiphase Condensation Cascade in Massive Galaxies, Groups, and Clusters","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":155,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Université de Montréal","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; Magyar Tudományos Akadémia; Generalitat Valenciana; Ministerio de Economía y Competitividad; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Halo; Turbulence; Galaxy; Line (geometry); Molecular cloud; Velocity dispersion; Accretion (finance); Cascade; Field line","score_opus":0.009984820521387047,"score_gpt":0.2417894278693248,"score_spread":0.23180460734793776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2759719452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99028534,0.00004996134,0.008146668,0.000037708014,0.000006471693,0.000012421698,0.00040516283,0.00020495306,0.00085120864],"genre_scores_gemma":[0.9962788,0.00001252432,0.0033858633,0.00000621854,0.000006519386,0.000006346235,0.00019528597,0.000016634853,0.000091809234],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993896,0.000018943832,0.0000021085089,0.000012904793,0.000013047923,0.000014035433],"domain_scores_gemma":[0.9996705,0.00006377123,0.0000763814,0.000061646424,0.00003343887,0.000094177245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002549923,0.00015936379,0.0001842095,0.0009712822,0.00023667228,0.00056997745,0.00039391135,0.00020546226,0.0008962234],"category_scores_gemma":[0.0008686685,0.000116221054,0.00021738415,0.00054705003,0.00030384466,0.00035268953,0.00052756915,0.00020737787,0.0000963248],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040966412,0.00018935821,0.58880216,0.00004710034,0.00028476992,0.0002361339,0.00062878785,0.33224544,0.03983114,0.010396631,0.0011808035,0.02574804],"study_design_scores_gemma":[0.000032664746,0.000055683005,0.1388092,0.0000073307206,0.000015520585,0.000026571297,0.00013481903,0.85376436,0.0031224736,0.0032337331,0.0007805797,0.000017084047],"about_ca_topic_score_codex":0.007815992,"about_ca_topic_score_gemma":0.008330321,"teacher_disagreement_score":0.007815992,"about_ca_system_score_codex":0.00041616982,"about_ca_system_score_gemma":0.00020686719,"threshold_uncertainty_score":0.015540957},"labels":[],"label_agreement":null},{"id":"W2759839182","doi":"10.3847/1538-4357/aa8e4f","title":"Characterizing the Cloud Decks of Luhman 16AB with Medium-resolution Spectroscopic Monitoring<sup>∗</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Atmosphere (unit); Absorption (acoustics); Amplitude; Astrophysics; Spectral line; Absorption spectroscopy; Spectral resolution; Environmental science; Materials science; Atmospheric sciences; Physics; Analytical Chemistry (journal); Computational physics; Optics; Chemistry; Meteorology; Astronomy","score_opus":0.014092426789781952,"score_gpt":0.2430259032103583,"score_spread":0.22893347642057635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2759839182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989085,0.0000398739,0.00012144343,0.000009963447,0.0000019004077,0.0000046362534,0.00054980844,0.000012268767,0.00035165314],"genre_scores_gemma":[0.99810576,0.00002090569,0.0005105631,0.000016084414,0.0000045943953,0.000007682146,0.0011396866,0.000009608849,0.00018507865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999267,0.000006585877,0.0000028289114,0.000024839252,0.000016994818,0.000021942691],"domain_scores_gemma":[0.99978524,0.000022498543,0.00006910972,0.000020647083,0.000039256458,0.00006330842],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013623456,0.00015596065,0.00015025875,0.0003828417,0.00032500207,0.00023426152,0.00026008548,0.00016557635,0.0007882779],"category_scores_gemma":[0.00020939199,0.000111951806,0.00016388764,0.00028395402,0.00017207107,0.00010892891,0.00030393593,0.00016102508,0.00037485224],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033244633,0.000060468596,0.8892041,0.000030582247,0.000058953658,0.00021856782,0.0003517889,0.0006367645,0.09852933,0.000067339395,0.00030422097,0.010205416],"study_design_scores_gemma":[0.0000030783162,0.00002425767,0.99756926,0.0000023862774,0.0000070333513,0.00006132121,0.00007052639,0.0005297741,0.0013909937,0.00001602845,0.0003227051,0.0000025586035],"about_ca_topic_score_codex":0.014029842,"about_ca_topic_score_gemma":0.038284708,"teacher_disagreement_score":0.014029842,"about_ca_system_score_codex":0.00029566916,"about_ca_system_score_gemma":0.00010120798,"threshold_uncertainty_score":0.027896345},"labels":[],"label_agreement":null},{"id":"W2760591947","doi":"10.3847/1538-4357/aa8df3","title":"The Interstellar Medium in [O iii]-selected Star-forming Galaxies at z ∼ 3.2","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Science and Technology Facilities Council; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Interstellar medium; Galaxy; Metallicity; Ionization; Spectroscopy; Luminous infrared galaxy; Photoionization; Interstellar cloud","score_opus":0.008239397996273809,"score_gpt":0.22020611693387085,"score_spread":0.21196671893759705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2760591947","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985752,0.000116308285,0.00013808842,0.000017820708,0.0000020519483,0.000002279124,0.00027552588,0.000019814135,0.00085295475],"genre_scores_gemma":[0.9991761,0.000045219982,0.00010111737,0.000022235556,0.0000035631622,0.000002666383,0.00043120683,0.000006850924,0.00021101839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999254,0.000005174181,0.0000028810025,0.000022798618,0.000010621711,0.000033216427],"domain_scores_gemma":[0.9997472,0.000025697404,0.000082585895,0.00001321547,0.000026482474,0.00010487256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015187105,0.00021715296,0.00020424287,0.00095925137,0.00026350576,0.00051565556,0.00020419399,0.00021985378,0.0013478474],"category_scores_gemma":[0.00017593185,0.00013868994,0.00019768483,0.0004405527,0.00017652854,0.00025977078,0.00034278148,0.00023517753,0.00033663897],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041734046,0.00008340106,0.8921777,0.000020634274,0.00007219632,0.00029247822,0.0002355408,0.00024413361,0.10111989,0.00012007667,0.00043648444,0.0047800844],"study_design_scores_gemma":[0.0000038686226,0.0000172506,0.99769884,0.0000024324472,0.000013347977,0.000081045284,0.00007484249,0.00023212325,0.0016044297,0.000028839166,0.0002403806,0.0000026073167],"about_ca_topic_score_codex":0.0046099857,"about_ca_topic_score_gemma":0.006847402,"teacher_disagreement_score":0.0046099857,"about_ca_system_score_codex":0.00022008471,"about_ca_system_score_gemma":0.000063106374,"threshold_uncertainty_score":0.0091663},"labels":[],"label_agreement":null},{"id":"W2760959279","doi":"10.3847/1538-4357/aa961b","title":"Evidence of Absence of Tidal Features in the Outskirts of Ultra Diffuse Galaxies in the Coma Cluster","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Coma Cluster; Surface brightness; Galaxy; RADIUS; Coma (optics); Position angle; Virgo Cluster; Effective radius","score_opus":0.01505798398593719,"score_gpt":0.2524972952803291,"score_spread":0.2374393112943919,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2760959279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99959296,0.000026214018,0.00009190362,0.0000038229023,6.3130096e-7,8.415159e-7,0.00006158136,0.0000112093985,0.00021095047],"genre_scores_gemma":[0.9997639,0.0000081450335,0.00004965973,0.000002099524,0.0000011370738,4.7669792e-7,0.00013100452,0.0000023851837,0.000041074145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979335,0.000015988835,0.000010961573,0.000049329174,0.000044928864,0.000085498075],"domain_scores_gemma":[0.9987394,0.00009862115,0.00033567363,0.00018018173,0.00017043101,0.00047574897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018695129,0.00026659426,0.00035764408,0.0013227963,0.0005250326,0.00080456916,0.00036180124,0.00018151483,0.0009301472],"category_scores_gemma":[0.0007386007,0.00027942425,0.00025804184,0.000872297,0.00055510626,0.00028755396,0.00079183135,0.00019639565,0.0002030642],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030297987,0.000030325926,0.96748114,0.000017393619,0.00008051147,0.0002157942,0.00041296196,0.00055979163,0.027489208,0.00016846911,0.00012398379,0.0031173637],"study_design_scores_gemma":[0.0000018268495,0.000023495151,0.9983741,0.0000014554223,0.000011817179,0.00006543002,0.000115740964,0.00038992622,0.0009080152,0.000027248147,0.00007747535,0.0000034719358],"about_ca_topic_score_codex":0.0103317695,"about_ca_topic_score_gemma":0.010517423,"teacher_disagreement_score":0.0103317695,"about_ca_system_score_codex":0.000355573,"about_ca_system_score_gemma":0.00020629223,"threshold_uncertainty_score":0.020543277},"labels":[],"label_agreement":null},{"id":"W2761014150","doi":"10.3847/1538-4357/aa9221","title":"Self-consistent Bulge/Disk/Halo Galaxy Dynamical Modeling Using Integral Field Kinematics","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Australian Research Council; Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Stellar kinematics; Galaxy; Bulge; Velocity dispersion; Dark matter; Kinematics; Galaxy rotation curve; Spiral galaxy; Surface brightness; Dark matter halo; Galaxy formation and evolution; Halo; Milky Way; Classical mechanics","score_opus":0.016563415333264747,"score_gpt":0.2475270456682179,"score_spread":0.23096363033495315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761014150","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1176268,0.0001574962,0.8748989,0.00011194138,0.000035856836,0.00005172315,0.0005199767,0.0012391829,0.005358058],"genre_scores_gemma":[0.7792115,0.00019812195,0.21416594,0.00008929699,0.00006187693,0.00015528823,0.00066857366,0.0005200046,0.0049293605],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998796,0.000035352703,0.0000063772923,0.00002829843,0.00002856687,0.00002173518],"domain_scores_gemma":[0.9996207,0.00012097277,0.0000684658,0.00007479867,0.000070668386,0.000044316323],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005377431,0.0005329885,0.0004362533,0.00095902564,0.000434175,0.00088387926,0.0016270223,0.0006061849,0.0026797543],"category_scores_gemma":[0.0013415874,0.00048844854,0.0009288843,0.00038777152,0.00050988013,0.0007534422,0.00065907865,0.0004269085,0.000584461],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000014679166,0.000016075743,0.003833007,0.000010970695,0.000022161095,0.000049093684,0.000036931197,0.979652,0.0009453913,0.008966878,0.00030454178,0.0061483155],"study_design_scores_gemma":[0.0000021642827,0.0000022277986,0.00013270242,0.0000020708096,0.0000020169812,0.000008348658,0.0000031363593,0.9977246,0.0001501526,0.0016063084,0.00036371077,0.0000025420165],"about_ca_topic_score_codex":0.017485816,"about_ca_topic_score_gemma":0.011460166,"teacher_disagreement_score":0.017485816,"about_ca_system_score_codex":0.0009493735,"about_ca_system_score_gemma":0.00089379173,"threshold_uncertainty_score":0.034768105},"labels":[],"label_agreement":null},{"id":"W2761580237","doi":"10.3847/0004-637x/830/2/97","title":"ACTION-BASED DYNAMICAL MODELING FOR THE MILKY WAY DISK","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Stars; Gravitational potential; Rotational symmetry; Parameterized complexity; Function (biology); Proper motion; Computational astrophysics","score_opus":0.0205043075921014,"score_gpt":0.249340287123852,"score_spread":0.2288359795317506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761580237","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.40053648,0.00059751933,0.5891055,0.0007374464,0.000034816436,0.00008088852,0.0008717779,0.00086422596,0.0071714604],"genre_scores_gemma":[0.96360683,0.00015720182,0.033478133,0.00007512468,0.00002449241,0.00009312717,0.00047568226,0.00013163808,0.0019578615],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980575,0.00007877459,0.000009321724,0.000045845776,0.00003584307,0.000024516434],"domain_scores_gemma":[0.99901545,0.000527551,0.0001453664,0.00012214946,0.00009667673,0.00009268079],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066975533,0.000415719,0.000516941,0.0006912246,0.0004109894,0.0009135451,0.001438367,0.0008730586,0.0020054185],"category_scores_gemma":[0.0037203366,0.00032799836,0.0008626358,0.0003401262,0.00075604045,0.0010063507,0.0012901803,0.0005297417,0.00032832593],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00001925276,0.000007703261,0.0018964094,0.000015865886,0.00002022797,0.000066338056,0.000068845075,0.97652656,0.00039665148,0.018083349,0.00020554756,0.0026932242],"study_design_scores_gemma":[0.0000026488635,0.0000034532213,0.00021727312,0.0000018091835,0.0000014025463,0.000009498529,0.000005775771,0.99419135,0.000044529217,0.005238105,0.00028124094,0.0000029253217],"about_ca_topic_score_codex":0.0130558275,"about_ca_topic_score_gemma":0.004705504,"teacher_disagreement_score":0.0130558275,"about_ca_system_score_codex":0.0009395866,"about_ca_system_score_gemma":0.00059471204,"threshold_uncertainty_score":0.02595967},"labels":[],"label_agreement":null},{"id":"W2761665501","doi":"10.3847/1538-4357/aa921b","title":"A Wide Dispersion in Star Formation Rate and Dynamical Mass of 10<sup>8</sup> Solar Mass Black Hole Host Galaxies at Redshift 6","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Galaxy; Star formation; Redshift; Velocity dispersion; Solar mass; Black hole (networking); Metallicity; Supermassive black hole","score_opus":0.006692504712230077,"score_gpt":0.20825240639927714,"score_spread":0.20155990168704707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761665501","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991322,0.000051890966,0.0000614987,0.000010005742,0.0000010002311,0.000002129397,0.0003086181,0.0000063948437,0.0004264573],"genre_scores_gemma":[0.9992625,0.000017492957,0.000056926478,0.0000054177735,0.0000031054742,0.0000012767615,0.00048825462,0.0000015749443,0.00016338332],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984825,0.00001758097,0.000015594187,0.000045309735,0.000036843652,0.000036410558],"domain_scores_gemma":[0.99912626,0.00016028722,0.00038089475,0.00007355524,0.00009219227,0.00016683375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025113914,0.00014071607,0.00018616505,0.0010145386,0.00020014777,0.0005524031,0.00021232828,0.00015938735,0.0017158231],"category_scores_gemma":[0.0005402296,0.00008874018,0.00011756688,0.00053637684,0.00020453519,0.00025782126,0.00036824858,0.00012503646,0.00036857772],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005775429,0.00002126561,0.991288,0.0000059988756,0.000018488097,0.000055813834,0.00014427197,0.00005741255,0.005627005,0.00005743999,0.000070292364,0.0025962244],"study_design_scores_gemma":[7.226533e-7,0.000013178192,0.9995679,5.475847e-7,0.0000026295072,0.000062275874,0.000036964368,0.00005630827,0.00017119964,0.0000074345025,0.00008014369,6.428815e-7],"about_ca_topic_score_codex":0.0012418211,"about_ca_topic_score_gemma":0.0021052845,"teacher_disagreement_score":0.0017158231,"about_ca_system_score_codex":0.00012248803,"about_ca_system_score_gemma":0.0000456818,"threshold_uncertainty_score":0.0057399273},"labels":[],"label_agreement":null},{"id":"W2761926605","doi":"10.1088/0004-637x/721/2/1193","title":"THE EVOLUTION OF PSR J0737–3039B AND A MODEL FOR RELATIVISTIC SPIN PRECESSION","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Precession; Flux (metallurgy); Pulse (music); Beam (structure); Spin (aerodynamics); Millisecond pulsar; Relativistic beaming","score_opus":0.010702874832225397,"score_gpt":0.3360622697877756,"score_spread":0.3253593949555502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761926605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9873439,0.0010053667,0.0022775184,0.000532978,0.000041349304,0.000023563043,0.0010505203,0.00018450936,0.0075404155],"genre_scores_gemma":[0.9962291,0.00024481805,0.001324408,0.0000789326,0.000025706388,0.000016442646,0.0012578756,0.000076850425,0.00074580335],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998661,0.00002056674,0.0000076676815,0.00004010565,0.000025341471,0.000040113224],"domain_scores_gemma":[0.9996189,0.000058358586,0.00012312391,0.000053457992,0.000058387704,0.000087804176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004904666,0.0006136687,0.0006061716,0.0013202934,0.00066267315,0.0011793312,0.00082661834,0.0010639238,0.0015348347],"category_scores_gemma":[0.0010066984,0.0003845917,0.00066498417,0.0012847859,0.0007373165,0.0005765702,0.00062589045,0.0005801293,0.0009232998],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007901855,0.0003210656,0.64781845,0.0002950076,0.0003412592,0.0039164205,0.0010570147,0.1926144,0.07282729,0.033475984,0.011512762,0.035030216],"study_design_scores_gemma":[0.00014563005,0.00017697396,0.5669649,0.00007029501,0.0001311659,0.001586028,0.00031921075,0.41055694,0.002934838,0.008165302,0.008813002,0.00013565687],"about_ca_topic_score_codex":0.039741825,"about_ca_topic_score_gemma":0.019013744,"teacher_disagreement_score":0.039741825,"about_ca_system_score_codex":0.0026436537,"about_ca_system_score_gemma":0.0007402506,"threshold_uncertainty_score":0.07902098},"labels":[],"label_agreement":null},{"id":"W2761937988","doi":"10.3847/1538-4357/aa9225","title":"The JCMT Transient Survey: Identifying Submillimeter Continuum Variability over Several Year Timescales Using Archival JCMT Gould Belt Survey Observations","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Protostar; Observable; Brightness; Sky; James Clerk Maxwell Telescope; Amplitude; Large Synoptic Survey Telescope; Star formation; Variable star","score_opus":0.07181006782219881,"score_gpt":0.3064226638324838,"score_spread":0.23461259601028497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2761937988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932389,0.00007699508,0.0010944341,0.0000519011,0.000006509654,0.000042567866,0.0038396802,0.00020263228,0.0014462444],"genre_scores_gemma":[0.99173415,0.000054188626,0.0026720073,0.000047928133,0.000024901878,0.00004194183,0.004981371,0.00004599999,0.00039745358],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997044,0.000024623463,0.00001681243,0.0000817856,0.00010780574,0.00006449966],"domain_scores_gemma":[0.9975752,0.00023581892,0.0010520151,0.00040633595,0.00032999643,0.00040064985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061288604,0.00015379289,0.00021200196,0.0029059378,0.00042477122,0.000688259,0.0004241594,0.0002466772,0.0011169934],"category_scores_gemma":[0.0016104799,0.0001374018,0.00026419098,0.002281115,0.00020811631,0.0003558073,0.00059554836,0.00021176883,0.00033764917],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010093264,0.000046155274,0.9742536,0.000027683329,0.000047235262,0.00016322102,0.00029199422,0.00038342478,0.0099577475,0.00010757296,0.0020632076,0.012557197],"study_design_scores_gemma":[0.0000028179995,0.0000074951477,0.9982198,0.0000028568923,0.0000069135117,0.000036084435,0.000047929276,0.00061028113,0.0003956957,0.000013958781,0.00065387593,0.0000022499494],"about_ca_topic_score_codex":0.032357313,"about_ca_topic_score_gemma":0.063037336,"teacher_disagreement_score":0.032357313,"about_ca_system_score_codex":0.0005981253,"about_ca_system_score_gemma":0.00034982243,"threshold_uncertainty_score":0.06433791},"labels":[],"label_agreement":null},{"id":"W2762143609","doi":"10.3847/1538-4357/aaa0da","title":"The Impact of Baryonic Physics on the Kinetic Sunyaev–Zel’dovich Effect","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Sunyaev–Zel'dovich effect; Baryon; Kinetic energy; Astrophysics; Galaxy; Spectral density; Electron; Reionization; Galaxy cluster; Redshift; Quantum mechanics; Statistics","score_opus":0.006470465253936855,"score_gpt":0.23703034097360703,"score_spread":0.23055987571967018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2762143609","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99237275,0.000092713366,0.0027389952,0.0003329287,0.000018040004,0.000009805794,0.00015050803,0.0001592706,0.004125149],"genre_scores_gemma":[0.99928087,0.000021381828,0.00036898008,0.00003724838,0.0000051065113,0.0000033019232,0.000056030403,0.00003145936,0.00019562781],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980575,0.000055974044,0.000007763164,0.000025325373,0.000040951953,0.00006427292],"domain_scores_gemma":[0.9987078,0.00073151407,0.00016757006,0.00011536292,0.00007982698,0.00019799564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007409962,0.00034671044,0.0004824384,0.00045630353,0.00045803643,0.00092315907,0.00081098906,0.00044221614,0.0018065803],"category_scores_gemma":[0.003971106,0.00027927323,0.000463073,0.0002651365,0.00086501776,0.0005438477,0.00068205193,0.00069703895,0.00014903687],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027988935,0.000099996156,0.105898984,0.00007607517,0.00019643232,0.00037573717,0.00018285163,0.8659141,0.010255865,0.010907222,0.0013112003,0.0045016045],"study_design_scores_gemma":[0.000101420854,0.00007315137,0.044166375,0.000015829766,0.000026628708,0.000054688866,0.00006786462,0.94866914,0.0036416592,0.0025964235,0.0005550593,0.0000317894],"about_ca_topic_score_codex":0.014432122,"about_ca_topic_score_gemma":0.0076425644,"teacher_disagreement_score":0.014432122,"about_ca_system_score_codex":0.00075979077,"about_ca_system_score_gemma":0.0004956753,"threshold_uncertainty_score":0.028696239},"labels":[],"label_agreement":null},{"id":"W2762456709","doi":"10.3847/1538-4357/aab6b1","title":"Measuring Dark Energy Properties with Photometrically Classified Pan-STARRS Supernovae. II. Cosmological Parameters","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; FAS Division of Science, Harvard University; Australian Astronomical Optics-Macquarie; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Centre National de la Recherche Scientifique; Ministério da Ciência, Tecnologia e Inovação; Centre National d’Etudes Spatiales; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Vanderbilt University; University of Chicago; Harvard University; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; New Mexico State University; University of Portsmouth; Yale University; National Science Foundation","keywords":"Physics; Cosmic microwave background; Dark energy; Astrophysics; Supernova; Redshift; Planck; Luminosity; Cosmology; Galaxy; Astronomy","score_opus":0.03938492794639218,"score_gpt":0.21807205436524493,"score_spread":0.17868712641885276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2762456709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978211,0.000041324714,0.001134578,0.000005375214,0.0000015498933,0.0000055949804,0.00044480615,0.000027726672,0.0005178802],"genre_scores_gemma":[0.99779993,0.000020552035,0.0010177115,0.0000035243643,0.0000019529207,0.000003357204,0.0010311585,0.000006062454,0.000115780356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960893,0.00010598345,0.00003938234,0.00010070395,0.00011038164,0.00003476639],"domain_scores_gemma":[0.9983486,0.00033236414,0.0007039233,0.00030955527,0.00017848867,0.00012705903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012741339,0.00038947037,0.00025022493,0.0014676446,0.00021746707,0.00058572274,0.00031683932,0.00020306188,0.0007937828],"category_scores_gemma":[0.0024055797,0.00024248377,0.00033965506,0.0011186982,0.00026369776,0.00043172596,0.00050872256,0.00020796219,0.00024421696],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006405106,0.00002155906,0.99130476,0.000009438158,0.00007041432,0.000011561644,0.000026735363,0.0020395685,0.00204639,0.00015060551,0.000052830663,0.0042021717],"study_design_scores_gemma":[0.000003942865,0.00004578087,0.98935753,0.000003966823,0.000020153988,0.000059574424,0.000036641744,0.007212515,0.00280325,0.00018106667,0.00026887955,0.0000066149246],"about_ca_topic_score_codex":0.003726765,"about_ca_topic_score_gemma":0.009462288,"teacher_disagreement_score":0.003726765,"about_ca_system_score_codex":0.0002953297,"about_ca_system_score_gemma":0.00012583449,"threshold_uncertainty_score":0.007410109},"labels":[],"label_agreement":null},{"id":"W2763117186","doi":"10.3847/1538-4357/aab9bb","title":"The Complete Light-curve Sample of Spectroscopically Confirmed SNe Ia from Pan-STARRS1 and Cosmological Constraints from the Combined Pantheon Sample","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2765,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; National Central University; Queen's University; Ministerio de Ciencia, Tecnología e Innovación Productiva; Space Telescope Science Institute; Office of Science; Johns Hopkins University; Queen's University Belfast; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; U.S. Department of Energy; Comisión Nacional de Investigación Científica y Tecnológica; University of Chicago; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Cosmic microwave background; Redshift; Photometry (optics); Dark energy; Light curve; Planck; Omega; Supernova; Cosmology; Cosmic distance ladder; Astronomy; Galaxy; Stars; Optics","score_opus":0.016602411439490386,"score_gpt":0.2451809563416259,"score_spread":0.22857854490213553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2763117186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99508095,0.00009549286,0.0002925578,0.00004064927,0.000003162972,0.000017646387,0.002435508,0.000023233284,0.0020107445],"genre_scores_gemma":[0.9864602,0.00016194544,0.000660116,0.00004100511,0.000017943024,0.000030276793,0.011203127,0.000024354249,0.0014009958],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99941754,0.000098815064,0.00003197957,0.00016016996,0.0001948353,0.00009682178],"domain_scores_gemma":[0.9990243,0.00013010831,0.00023754544,0.00023957525,0.00018944085,0.00017895541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007393647,0.0003072116,0.00037191832,0.0016236162,0.00029115236,0.00042158554,0.0003256773,0.00014744104,0.0039898595],"category_scores_gemma":[0.0013574827,0.00021940148,0.00027649247,0.0009477924,0.00019009005,0.0004154328,0.0011066619,0.00020280298,0.00087571045],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036242214,0.000050909264,0.96276987,0.000054223754,0.00009892085,0.00020536048,0.00029026665,0.0002347367,0.0060618888,0.00026519745,0.0022925497,0.027313655],"study_design_scores_gemma":[0.000008818434,0.000030925887,0.99628097,0.0000055903206,0.00001557915,0.00022920391,0.00009174116,0.0002560024,0.0004468601,0.00003201939,0.0025992736,0.0000030663264],"about_ca_topic_score_codex":0.0047955676,"about_ca_topic_score_gemma":0.014746962,"teacher_disagreement_score":0.0047955676,"about_ca_system_score_codex":0.00024289126,"about_ca_system_score_gemma":0.00028282357,"threshold_uncertainty_score":0.013347387},"labels":[],"label_agreement":null},{"id":"W2763201488","doi":"10.3847/1538-4357/aa9185","title":"Physical Properties of 15 Quasars at z ≳ 6.5","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":316,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of California, Los Angeles; Jet Propulsion Laboratory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Astronomical Observatory of Japan; National Central University; Durham University; Istituto Nazionale di Astrofisica; W. M. Keck Foundation; Centre National de la Recherche Scientifique; Deutsche Forschungsgemeinschaft; Queen's University Belfast; Smithsonian Institution; National Radio Astronomy Observatory; Agence Nationale de la Recherche; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; National Science Council; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; National Institutes of Natural Sciences; Universität Heidelberg; Leibniz-Gemeinschaft; University of Notre Dame; Johns Hopkins University; Queen's University; Ohio State University; Max-Planck-Gesellschaft; National Science Foundation; University of Minnesota; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Quasar; Astrophysics; Astronomy; Galaxy","score_opus":0.015289566804003079,"score_gpt":0.2273462553629047,"score_spread":0.2120566885589016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2763201488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99958295,0.000032223303,0.000034804238,0.0000046330606,0.0000011452504,0.0000034251007,0.00020417581,0.000004245231,0.00013230933],"genre_scores_gemma":[0.99918705,0.000027606791,0.00006196535,0.0000069683238,0.0000061505566,0.0000033219053,0.0005525622,0.0000012610719,0.00015304968],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983776,0.000018976089,0.000016930253,0.000046630827,0.0000309932,0.000048704125],"domain_scores_gemma":[0.99914765,0.00010778538,0.00033199348,0.000047323298,0.00009771589,0.00026766252],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040205746,0.00032208933,0.00026780152,0.0010979882,0.00027090087,0.000528756,0.00023149983,0.0002622533,0.0011050407],"category_scores_gemma":[0.0005986711,0.00014568576,0.00022616876,0.0006150775,0.00026724703,0.00028221213,0.00033196944,0.00017644004,0.0003358496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049217477,0.000047976137,0.9961815,0.0000047472013,0.000019382447,0.00007037409,0.00012580644,0.00006151282,0.001985267,0.00001754465,0.00005435797,0.0013823909],"study_design_scores_gemma":[0.00000206948,0.00010562664,0.99926287,0.0000010165234,0.00000623223,0.00011775247,0.000079378005,0.00009418033,0.00019301267,0.0000064733536,0.0001298847,0.0000015827156],"about_ca_topic_score_codex":0.0020341326,"about_ca_topic_score_gemma":0.001331187,"teacher_disagreement_score":0.0020341326,"about_ca_system_score_codex":0.000127839,"about_ca_system_score_gemma":0.000060784867,"threshold_uncertainty_score":0.0040445924},"labels":[],"label_agreement":null},{"id":"W2763628561","doi":"10.3847/1538-4357/aa8f44","title":"Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy cluster; Globular cluster; Brightest cluster galaxy; Galaxy; Cluster (spacecraft); Luminosity; Elliptical galaxy; Galaxy group","score_opus":0.009389407646069358,"score_gpt":0.21102176635531042,"score_spread":0.20163235870924107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2763628561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982248,0.000035707028,0.00038543774,0.000016933047,0.0000015854397,0.000002661927,0.00060608843,0.000069353155,0.0006574239],"genre_scores_gemma":[0.99786586,0.00001616584,0.00052694016,0.000008239634,0.0000018821636,0.000004230073,0.0012452214,0.00002101343,0.00031050167],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992144,0.0000068665113,0.000003534442,0.000027020888,0.0000195876,0.00002159188],"domain_scores_gemma":[0.999734,0.00003497381,0.00008684943,0.00002361365,0.00004354184,0.00007708858],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011883748,0.00021110577,0.00023381347,0.0010239478,0.00023048453,0.00034087396,0.00020479961,0.00021638801,0.0016511958],"category_scores_gemma":[0.0003888686,0.00014503016,0.00024476944,0.00047353894,0.00012310887,0.0001767817,0.00027749338,0.0001676318,0.0005131659],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018437442,0.000045813566,0.93940085,0.000029769322,0.00006806024,0.00014102343,0.00027184584,0.004372443,0.043179076,0.00032305883,0.0011033512,0.010880307],"study_design_scores_gemma":[0.0000031903096,0.000015789874,0.99385744,0.0000029910739,0.0000066344182,0.00005044031,0.00006683057,0.004047797,0.0013553691,0.00008425117,0.0005035997,0.000005668077],"about_ca_topic_score_codex":0.011251036,"about_ca_topic_score_gemma":0.016423747,"teacher_disagreement_score":0.011251036,"about_ca_system_score_codex":0.0004006737,"about_ca_system_score_gemma":0.000094153795,"threshold_uncertainty_score":0.022371113},"labels":[],"label_agreement":null},{"id":"W2763987867","doi":"10.3847/1538-4357/aa9180","title":"Discovery of Diffuse Dwarf Galaxy Candidates around M101","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Surface brightness; Astrophysics; Galaxy; Luminosity; Milky Way; Dwarf galaxy; Brightness; Local Group; Luminosity function; Astronomy","score_opus":0.008829351415021893,"score_gpt":0.22662401934817908,"score_spread":0.2177946679331572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2763987867","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984236,0.000110748035,0.00029216506,0.000019646533,0.0000027159663,0.0000068737445,0.00012695788,0.00002086428,0.0009964952],"genre_scores_gemma":[0.9982109,0.000037945516,0.00064629456,0.000021434576,0.000003895334,0.0000034528425,0.00069443195,0.0000043336854,0.0003772883],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998498,0.0000162971,0.000009989712,0.000034831664,0.000054062366,0.000034983732],"domain_scores_gemma":[0.99935156,0.00008517504,0.00012630744,0.000071466886,0.000106417334,0.00025913664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025318484,0.0002536432,0.00028717262,0.0011583489,0.00055427174,0.0006692714,0.00043548047,0.00025145733,0.0012670284],"category_scores_gemma":[0.0005973664,0.00012196599,0.00017464737,0.000945792,0.00022679302,0.00018337113,0.0006715437,0.00021362302,0.00054503576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015956942,0.00008629874,0.95023286,0.00004710183,0.00003971675,0.00095261174,0.0004084303,0.00029365264,0.032924615,0.00022054015,0.00041479943,0.0142198065],"study_design_scores_gemma":[0.000010713616,0.0001803461,0.9904221,0.0000095053165,0.000023277935,0.00074650365,0.00040888935,0.0007334227,0.0046530594,0.00007219663,0.0027323277,0.000007683162],"about_ca_topic_score_codex":0.0052506835,"about_ca_topic_score_gemma":0.01102856,"teacher_disagreement_score":0.0052506835,"about_ca_system_score_codex":0.00043983455,"about_ca_system_score_gemma":0.00027290866,"threshold_uncertainty_score":0.01044023},"labels":[],"label_agreement":null},{"id":"W2764026501","doi":"10.3847/1538-4357/aa8a6f","title":"Uplift, Feedback, and Buoyancy: Radio Lobe Dynamics in NGC 4472","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Surface brightness; Erg; Galaxy; Radio galaxy; Lobe; Classification of discontinuities; Roche lobe; Brightness","score_opus":0.006401789025636335,"score_gpt":0.21471566753637286,"score_spread":0.20831387851073652,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2764026501","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995981,0.000042964137,0.000039956183,0.000011386621,0.0000010081076,9.565183e-7,0.00006211145,0.000019591242,0.0002239007],"genre_scores_gemma":[0.99974316,0.000011566796,0.00005822119,0.000004066093,0.0000024918284,0.000001230276,0.000078865494,0.0000037820794,0.00009666038],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991226,0.000007050933,0.0000028277218,0.000017845914,0.000022398888,0.00003761701],"domain_scores_gemma":[0.99968827,0.000046628793,0.000092490955,0.000029102293,0.000037506397,0.00010606365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110050314,0.00039686376,0.00035559115,0.0007685276,0.00050314085,0.00048205227,0.00039121145,0.0002854526,0.001345394],"category_scores_gemma":[0.00039074462,0.00020862077,0.00020332284,0.00044972595,0.00031980366,0.00022172525,0.0004603728,0.0002448432,0.00026286463],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00088963256,0.00017701156,0.7185963,0.00007014908,0.00011476477,0.0013434397,0.0007853687,0.0058772173,0.25812456,0.0002703592,0.00083516596,0.012916026],"study_design_scores_gemma":[0.0000102083095,0.000054680575,0.99590486,0.0000023948999,0.000014545978,0.00012228465,0.000103032056,0.0017520895,0.0016744914,0.000055448098,0.0002930344,0.000012910617],"about_ca_topic_score_codex":0.0165732,"about_ca_topic_score_gemma":0.017786853,"teacher_disagreement_score":0.0165732,"about_ca_system_score_codex":0.00050750084,"about_ca_system_score_gemma":0.0001278568,"threshold_uncertainty_score":0.03295344},"labels":[],"label_agreement":null},{"id":"W2764313219","doi":"10.3847/1538-4357/aa8c70","title":"Erratum: “A Measurement of the Cosmic Microwave Background B-Mode Polarization Power Spectrum at Sub-degree Scales with POLARBEAR” (2014, ApJ, 794, 171)","year":2017,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); McGill University; Dalhousie University","funders":"","keywords":"Physics; Cosmic microwave background; Polarization (electrochemistry); Spectral density; Spectrum (functional analysis); Astrophysics; Mode (computer interface); COSMIC cancer database; Microwave; Degree (music); Optics; Quantum mechanics; Statistics; Acoustics","score_opus":0.014576680539456826,"score_gpt":0.238356580291221,"score_spread":0.22377989975176418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2764313219","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0006707145,0.0007879953,0.0003667333,0.060407225,0.9220805,0.000024000467,0.0018802168,0.00039401662,0.013388595],"genre_scores_gemma":[0.016480496,0.0050564753,0.0029468348,0.10499175,0.24356796,0.00012285014,0.007876526,0.002002492,0.6169546],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99821126,0.00013719617,0.00031677613,0.0002485911,0.00092579215,0.00016042015],"domain_scores_gemma":[0.9932286,0.0011998424,0.00040958385,0.0005249185,0.0041963453,0.0004407811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015668329,0.0020252215,0.0012151471,0.0028479223,0.00514635,0.003477538,0.0024170005,0.0049374886,0.03812473],"category_scores_gemma":[0.015581183,0.0007841162,0.0010462337,0.0016642285,0.0021104037,0.0032558506,0.0020630772,0.007904367,0.033987705],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000026774645,0.000010642694,0.00010235335,0.000031116644,0.0000038714675,0.00018835737,0.000014803393,0.00002760168,0.000103854094,0.0006149204,0.9961898,0.0026858912],"study_design_scores_gemma":[0.000028849645,0.0000322244,0.0023309297,0.00017805927,0.000025479738,0.00042468298,0.00017793705,0.0002719044,0.0009946459,0.0020992148,0.99338466,0.00005142049],"about_ca_topic_score_codex":0.024184378,"about_ca_topic_score_gemma":0.032506913,"teacher_disagreement_score":0.03812473,"about_ca_system_score_codex":0.0038601698,"about_ca_system_score_gemma":0.004667373,"threshold_uncertainty_score":0.12753993},"labels":[],"label_agreement":null},{"id":"W2765458810","doi":"10.3847/1538-4357/aa96fd","title":"The Sleeping Monster: NuSTAR Observations of SGR 1806–20, 11 Years After the Giant Flare","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Flare; Flux (metallurgy); Bursting; Spectral line; Telescope; Noise (video); Magnetic dipole; Dipole; Light curve","score_opus":0.021438268422734136,"score_gpt":0.308326123987287,"score_spread":0.2868878555645529,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765458810","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998018,0.00010883874,0.00008741595,0.00003111272,0.000011720778,0.0000039492024,0.00082090753,0.000021540447,0.0008963643],"genre_scores_gemma":[0.9961521,0.00006141224,0.00022579302,0.000029841352,0.000024390065,0.00000393799,0.0030338778,0.000009616408,0.00045893595],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987566,0.000009910442,0.000010938226,0.000034343724,0.00004061631,0.000028430131],"domain_scores_gemma":[0.9995956,0.000024838462,0.0001525939,0.00004043756,0.000059905382,0.00012660085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027184677,0.00019993109,0.00031468057,0.0009021324,0.00039288448,0.0005001747,0.00023500987,0.00031044293,0.0006238602],"category_scores_gemma":[0.0005070903,0.000106722575,0.00029472072,0.00058766257,0.00022750255,0.00023070879,0.0005818612,0.0002800953,0.0003645105],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000546062,0.000092155875,0.9679718,0.000058042053,0.00011186704,0.0010644536,0.00073242874,0.00044029497,0.018323569,0.00011359499,0.0014023666,0.009143472],"study_design_scores_gemma":[0.0000045855654,0.00006796526,0.99730456,0.000007098999,0.000013689252,0.0002614342,0.00016884466,0.00022598483,0.0005856616,0.000017263577,0.0013371268,0.000005790245],"about_ca_topic_score_codex":0.007895129,"about_ca_topic_score_gemma":0.02527488,"teacher_disagreement_score":0.007895129,"about_ca_system_score_codex":0.0002981679,"about_ca_system_score_gemma":0.00022009814,"threshold_uncertainty_score":0.015698373},"labels":[],"label_agreement":null},{"id":"W2765538943","doi":"10.3847/1538-4357/ab229e","title":"Algorithms for FFT Beamforming Radio Interferometers","year":2019,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; University of Toronto; University of British Columbia","funders":"","keywords":"Beamforming; Astronomical interferometer; Fourier transform; Algorithm; Fast Fourier transform; Physics; Intensity mapping; Brightness; Sky; Computation; Computer science; Optics; Telecommunications; Interferometry; Astrophysics; Galaxy","score_opus":0.027216676917071206,"score_gpt":0.3434152794697358,"score_spread":0.31619860255266463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765538943","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011486892,0.000046004305,0.9973037,0.000050296,0.000023654806,0.00003142533,0.00006885966,0.00041426666,0.0009130366],"genre_scores_gemma":[0.04537431,0.00014674503,0.950928,0.000051622905,0.00006931335,0.00022305806,0.00051262666,0.00019969375,0.0024946893],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99910396,0.00019820382,0.00009625988,0.00014868696,0.00035500067,0.00009783228],"domain_scores_gemma":[0.9983962,0.00072574796,0.0001126888,0.00024144659,0.00047403594,0.000049872575],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011168991,0.0014516929,0.00073636504,0.0011950578,0.00064026355,0.0015576191,0.0014722288,0.0011003054,0.0141164465],"category_scores_gemma":[0.0062988107,0.0005021162,0.00084547856,0.0013561544,0.00068226294,0.0021018481,0.0016071415,0.0014863889,0.0066753593],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002140472,0.0000692134,0.001069195,0.00018877993,0.00004703188,0.0001443485,0.00016708506,0.25549325,0.013231251,0.14835717,0.009213772,0.57180494],"study_design_scores_gemma":[0.00003941974,0.000031746655,0.00017496769,0.000023656637,0.000006814015,0.00007503774,0.000041188952,0.9153469,0.0035729352,0.07483731,0.005831291,0.00001864669],"about_ca_topic_score_codex":0.0033477417,"about_ca_topic_score_gemma":0.00388072,"teacher_disagreement_score":0.0141164465,"about_ca_system_score_codex":0.00093219226,"about_ca_system_score_gemma":0.0011826144,"threshold_uncertainty_score":0.047224164},"labels":[],"label_agreement":null},{"id":"W2765568204","doi":"10.3847/1538-4357/aa974f","title":"Deep HST Imaging in 47 Tucanae: A Global Dynamical Model","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Globular cluster; Stellar dynamics; Subgiant; Velocity dispersion; Mass segregation; Stellar mass; Stars; Proper motion; RADIUS; Cluster (spacecraft)","score_opus":0.009368414439617266,"score_gpt":0.24782088817940867,"score_spread":0.2384524737397914,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765568204","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9934528,0.00019514494,0.0021427912,0.00046043933,0.000009467661,0.000015203012,0.0005937398,0.000051550403,0.0030789156],"genre_scores_gemma":[0.9979152,0.00010289689,0.00058529724,0.0000331685,0.000009730702,0.000012290793,0.0004460633,0.000018369727,0.0008768868],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998809,0.000008814038,0.0000031522993,0.000052702173,0.000011749355,0.000042625255],"domain_scores_gemma":[0.999851,0.000028522525,0.00002667333,0.000013408497,0.00003006374,0.000050360497],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030241095,0.00058064016,0.00057099614,0.00089699484,0.0014368676,0.0018349777,0.0013639436,0.0010867061,0.0019443007],"category_scores_gemma":[0.0005240743,0.00032192233,0.00072768383,0.0007162921,0.0011238304,0.00095285155,0.000783113,0.00043874368,0.00018847425],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019950615,0.00013323149,0.17138489,0.00005134939,0.000254208,0.0003739849,0.00038627617,0.79267925,0.008312389,0.0112544345,0.001979705,0.012990821],"study_design_scores_gemma":[0.000031034648,0.000034387947,0.09659395,0.000010503717,0.000088554196,0.000055564287,0.0002130704,0.89857084,0.00037730206,0.0027570769,0.0012314245,0.000036298297],"about_ca_topic_score_codex":0.38753656,"about_ca_topic_score_gemma":0.20376943,"teacher_disagreement_score":0.38753656,"about_ca_system_score_codex":0.0054813824,"about_ca_system_score_gemma":0.0019173039,"threshold_uncertainty_score":0.7705617},"labels":[],"label_agreement":null},{"id":"W2765598880","doi":"10.3847/1538-4357/aa94be","title":"Atomic Gas in Blue Ultra Diffuse Galaxies around Hickson Compact Groups","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Galaxy; Halo; Measure (data warehouse); Red shift; Galaxy group; Spin (aerodynamics)","score_opus":0.00881876502070312,"score_gpt":0.22131946693566987,"score_spread":0.21250070191496676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765598880","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99949074,0.00006385281,0.00007792128,0.0000060586067,8.631756e-7,0.0000012567399,0.000018308237,0.000004122016,0.00033684328],"genre_scores_gemma":[0.9998135,0.000016401988,0.00007352158,0.0000024183105,0.0000015837963,6.2137565e-7,0.00003452904,0.0000011983545,0.000056229474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990356,0.000011077017,0.0000032867995,0.000028237695,0.000023651195,0.000030212022],"domain_scores_gemma":[0.9994998,0.000072779454,0.00020262878,0.000046449142,0.000051836443,0.00012649037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025833945,0.00019703034,0.00019425723,0.0015306998,0.00031331877,0.00055302924,0.00030958347,0.00013929151,0.00072878523],"category_scores_gemma":[0.00064265606,0.000116044095,0.000073331306,0.0005714546,0.0004939441,0.00032083495,0.00076638954,0.00011511765,0.00010409425],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021011173,0.000031808977,0.9678151,0.000020722753,0.000043137275,0.00024459284,0.0010172536,0.0004662357,0.021383837,0.0006615467,0.00012965586,0.007975942],"study_design_scores_gemma":[0.0000063430357,0.000057289337,0.99512815,0.000009011669,0.00001896133,0.00018808937,0.00061848416,0.0008687544,0.0021907517,0.00022711136,0.0006815964,0.000005357181],"about_ca_topic_score_codex":0.0040269606,"about_ca_topic_score_gemma":0.004965406,"teacher_disagreement_score":0.0040269606,"about_ca_system_score_codex":0.00035593522,"about_ca_system_score_gemma":0.00006722328,"threshold_uncertainty_score":0.00800705},"labels":[],"label_agreement":null},{"id":"W2765742298","doi":"10.3847/1538-4357/aa901d","title":"Disentangling the Radio Emission of the Supernova Remnant W51C","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Supernova remnant; Maser; Milky Way; Near-Earth supernova; Supernova; Line (geometry); H II region; Spectral line; Magnetic field","score_opus":0.01166597925750266,"score_gpt":0.2379693087413151,"score_spread":0.22630332948381246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765742298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961105,0.000034287074,0.0009952638,0.00004221056,0.000009896048,0.000010615938,0.00021250838,0.000039889903,0.002544859],"genre_scores_gemma":[0.998475,0.00002200599,0.00059031695,0.000013775726,0.0000032190426,0.000010327229,0.00031988602,0.000017477505,0.00054798665],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999181,0.000019407526,0.0000035189555,0.000013378535,0.00001132303,0.000034248853],"domain_scores_gemma":[0.9996846,0.00011164608,0.00004676998,0.000035346613,0.00004282226,0.00007899749],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027916383,0.0003924641,0.0003890644,0.00036013604,0.00036908104,0.0007115768,0.00063641195,0.00055976433,0.0022627714],"category_scores_gemma":[0.0010662819,0.00024321847,0.0006029322,0.0003190314,0.00043665105,0.00036151885,0.0005919916,0.0003928117,0.00022181342],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033350653,0.000103435865,0.05102449,0.000022994858,0.00013991416,0.0004200438,0.00007129201,0.9405415,0.002742964,0.0023190698,0.0003410426,0.0019398178],"study_design_scores_gemma":[0.00013669897,0.00019434697,0.023447456,0.000010007058,0.00007520268,0.000067708075,0.00013127082,0.97313493,0.0012433557,0.0007584786,0.0007782104,0.000022381819],"about_ca_topic_score_codex":0.034354694,"about_ca_topic_score_gemma":0.022036389,"teacher_disagreement_score":0.034354694,"about_ca_system_score_codex":0.00064880226,"about_ca_system_score_gemma":0.00065418985,"threshold_uncertainty_score":0.06830943},"labels":[],"label_agreement":null},{"id":"W2765886468","doi":"10.3847/1538-4357/aabcba","title":"Demographics of Star-forming Galaxies since z ∼ 2.5. I. The UVJ Diagram in CANDELS","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Max-Planck-Institut für Astronomie; Centre National de la Recherche Scientifique; KU Leuven; Università degli Studi di Padova; Universidad Complutense de Madrid; University of California Observatories; Jet Propulsion Laboratory; Bundesministerium für Verkehr, Innovation und Technologie; Centre National d’Etudes Spatiales; Cardiff University; University of Sussex; National Science Foundation; Imperial College London; University of Lethbridge; California Institute of Technology; National Aeronautics and Space Administration; Space Telescope Science Institute; UK Space Agency","keywords":"Galaxy; Demographics; Diagram; Star formation; Population; Radio galaxy; Stellar population","score_opus":0.011886611744514488,"score_gpt":0.24780126720382378,"score_spread":0.23591465545930929,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765886468","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963167,0.00042986582,0.00015641942,0.000054122313,0.0000039861707,0.00000508426,0.00105635,0.00002815006,0.0019492471],"genre_scores_gemma":[0.9979056,0.00011961442,0.00015536121,0.000024736477,0.000006307359,0.0000040772566,0.0011876924,0.000007434636,0.00058926584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997501,0.000017957927,0.000017292845,0.00010235588,0.000038408576,0.00007392997],"domain_scores_gemma":[0.9984743,0.00012515098,0.00046044053,0.0001140564,0.00027030677,0.0005558265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005688285,0.00014948976,0.00022848097,0.003394471,0.0008315377,0.0012382547,0.00044606085,0.00023993106,0.0028785577],"category_scores_gemma":[0.0011729454,0.00010791231,0.0002696133,0.0018931347,0.0005148094,0.00074634864,0.0008924719,0.00028594944,0.00063494703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004913382,0.000010440164,0.9924493,0.000007864831,0.000009984102,0.000044361834,0.00026565723,0.0000703972,0.0005814353,0.0002985751,0.00020433475,0.006008645],"study_design_scores_gemma":[0.0000010409033,0.000015996813,0.99889576,0.000003931416,0.0000027250514,0.000056569188,0.0002263482,0.00007762613,0.00011422464,0.000054651242,0.00054823956,0.0000027699825],"about_ca_topic_score_codex":0.019853197,"about_ca_topic_score_gemma":0.021541676,"teacher_disagreement_score":0.019853197,"about_ca_system_score_codex":0.0005814983,"about_ca_system_score_gemma":0.00039254382,"threshold_uncertainty_score":0.039475262},"labels":[],"label_agreement":null},{"id":"W2765933318","doi":"10.3847/1538-4357/aaa54b","title":"The Origin of Molecular Clouds in Central Galaxies","year":2018,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Science and Technology Facilities Council; Canadian Space Agency; Smithsonian Institution","keywords":"Materials science","score_opus":0.0074903225038388645,"score_gpt":0.22289346528246892,"score_spread":0.21540314277863007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765933318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99882394,0.000321642,0.00008431925,0.000036674093,0.0000020121086,0.0000024093733,0.00012715615,0.000013282565,0.00058851327],"genre_scores_gemma":[0.99975747,0.000037893453,0.000025199115,0.000004930048,0.000002634288,7.1966076e-7,0.000079594945,0.0000015909494,0.00009003502],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996691,0.000040593433,0.000009418128,0.00006490314,0.000055826673,0.00016021974],"domain_scores_gemma":[0.9989127,0.00014780239,0.00037723052,0.00007307001,0.000116912066,0.00037224023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031914577,0.00022854676,0.00035616892,0.0021394275,0.0007258401,0.001559408,0.00039896904,0.00022379779,0.001511571],"category_scores_gemma":[0.0010868965,0.00021049414,0.00029182906,0.0015545423,0.0012195515,0.00033354768,0.00084445043,0.00025236738,0.00024876744],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009024792,0.000015009853,0.99298686,0.000012220591,0.00004757573,0.00011045118,0.00036918392,0.0002811677,0.0024726246,0.000739799,0.00020325255,0.002671526],"study_design_scores_gemma":[0.0000025475504,0.000010528292,0.9987729,0.0000047704934,0.000013084115,0.00004915604,0.00028148675,0.0002732906,0.00019610973,0.00008414111,0.00030930815,0.0000026367688],"about_ca_topic_score_codex":0.073093206,"about_ca_topic_score_gemma":0.05504849,"teacher_disagreement_score":0.073093206,"about_ca_system_score_codex":0.0013421586,"about_ca_system_score_gemma":0.00049914524,"threshold_uncertainty_score":0.1453355},"labels":[],"label_agreement":null},{"id":"W2765957322","doi":"10.3847/1538-4357/aa8d19","title":"Erratum: “Secure TTV Mass Measurements: Ten Kepler Exoplanets between 3 and 8 M<sub>⊕</sub> with Diverse Densities and Incident Fluxes” (2016, ApJ, 820, 39)","year":2017,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Bishop's University","funders":"","keywords":"Physics; Kepler; Exoplanet; Astrobiology; Astronomy; Astrophysics; Planet","score_opus":0.02334189327955655,"score_gpt":0.25234489296092477,"score_spread":0.22900299968136822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2765957322","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0023235367,0.0007814433,0.00073942536,0.065128945,0.89736295,0.000045239216,0.007229165,0.00080869783,0.025580594],"genre_scores_gemma":[0.040914077,0.0045851506,0.0064689447,0.08341691,0.15206634,0.00020568214,0.02653206,0.003523105,0.68228763],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9985318,0.00009795573,0.00027816114,0.00020518788,0.0007443552,0.00014247908],"domain_scores_gemma":[0.99375784,0.0011779671,0.00050188083,0.00058644486,0.0035787697,0.00039712395],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013206224,0.0016791398,0.0009949451,0.002203719,0.004459099,0.00276292,0.0019413595,0.0033262828,0.044637468],"category_scores_gemma":[0.015876139,0.00067499606,0.0007743233,0.0017162681,0.0015109737,0.0026143393,0.0021941857,0.005194737,0.03451788],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000044312677,0.000012354478,0.00027466798,0.00003683866,0.0000046015425,0.00023282773,0.00002959731,0.00004459728,0.00012614962,0.0005510646,0.9946195,0.004023476],"study_design_scores_gemma":[0.000037363214,0.000036817644,0.0036351404,0.00016368492,0.000027587372,0.00034313288,0.0003262897,0.00024906138,0.0012493442,0.0021047508,0.99177843,0.00004827211],"about_ca_topic_score_codex":0.022979239,"about_ca_topic_score_gemma":0.033390902,"teacher_disagreement_score":0.044637468,"about_ca_system_score_codex":0.002917411,"about_ca_system_score_gemma":0.004230573,"threshold_uncertainty_score":0.14932722},"labels":[],"label_agreement":null},{"id":"W2766247384","doi":"10.3847/1538-4357/aa93d7","title":"On the Origin of Banded Structure in Dusty Protoplanetary Disks: HL Tau and TW Hya","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Planetesimal; Planet; Physics; Protoplanetary disk; Context (archaeology); Population; Condensation; Astrophysics; Astrobiology; Planetary migration; Protoplanet; Circumstellar disk; Gravitation; Solar System; Planetary system; Astronomy; Geology; Paleontology","score_opus":0.013048119946633525,"score_gpt":0.25108136261924047,"score_spread":0.23803324267260695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766247384","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937433,0.00008867206,0.00012762043,0.000017251627,0.0000011575696,0.0000021891065,0.000019317038,0.0000031615502,0.00036633972],"genre_scores_gemma":[0.99989355,0.000014916714,0.00004405335,0.0000028921697,0.0000014597601,7.9604405e-7,0.000015046516,9.621842e-7,0.000026330781],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995923,0.000004603045,0.0000026562702,0.000012979023,0.000006618089,0.000013926385],"domain_scores_gemma":[0.999744,0.00005747828,0.00008099879,0.000019222576,0.00002377389,0.0000745105],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011785546,0.00015387402,0.00016228408,0.00052736077,0.0004299546,0.0007311768,0.00032756745,0.00036881812,0.00095036003],"category_scores_gemma":[0.00039430562,0.000118905155,0.00013912572,0.00026833056,0.0005589784,0.00036732244,0.00043984965,0.00019350077,0.00014684405],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005957184,0.00018029714,0.81625617,0.00006384141,0.00006847198,0.0017522869,0.0009806162,0.0032222143,0.16616592,0.0026891688,0.00019284633,0.007832445],"study_design_scores_gemma":[0.000023429524,0.00008096437,0.9815834,0.000008604834,0.000026827622,0.00056150614,0.00054312684,0.011286001,0.0046014325,0.0008607806,0.0004155623,0.000008332619],"about_ca_topic_score_codex":0.0021294106,"about_ca_topic_score_gemma":0.0015614132,"teacher_disagreement_score":0.0021294106,"about_ca_system_score_codex":0.00045784327,"about_ca_system_score_gemma":0.000085378415,"threshold_uncertainty_score":0.0042340755},"labels":[],"label_agreement":null},{"id":"W2766252874","doi":"10.3847/1538-4357/aa8e99","title":"Far-infrared to Millimeter Data of Protoplanetary Disks: Dust Growth in the Taurus, Ophiuchus, and Chamaeleon I Star-forming Regions<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Ophiuchus; Millimeter; Astrophysics; Physics; Opacity; Protoplanetary disk; Spectral index; Planet; Wavelength; Astronomy; Stars; Spectral line; Star formation; Optics","score_opus":0.03155208700383219,"score_gpt":0.2686100382124148,"score_spread":0.2370579512085826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766252874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981774,0.000056741308,0.00032481208,0.00001411385,0.0000010975436,0.0000023500818,0.0008536763,0.000019699073,0.0005500619],"genre_scores_gemma":[0.9980457,0.00002792514,0.0005477414,0.0000048115976,0.000004769698,0.0000029953544,0.0012625944,0.000005612681,0.00009774198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999113,0.0000121367075,0.000007193073,0.0000252998,0.000027816197,0.000016375987],"domain_scores_gemma":[0.99926525,0.00029106752,0.00022348935,0.00006691336,0.00008707985,0.00006626821],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025395924,0.0002130167,0.00015913662,0.0010683241,0.000149346,0.0004461418,0.00019058226,0.00019048777,0.0009951066],"category_scores_gemma":[0.0007859729,0.00011477282,0.00023816105,0.00080288417,0.00011743937,0.0002585627,0.00024135427,0.00014731583,0.00031791104],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011363229,0.00001436979,0.9845694,0.000015926673,0.00004601794,0.00004347262,0.00008731572,0.001432679,0.0066241543,0.00007864678,0.00013378423,0.0068405666],"study_design_scores_gemma":[0.0000014958638,0.00001018691,0.9979849,0.0000015082028,0.000008575572,0.00003536434,0.00006131255,0.0011019006,0.00060575764,0.00002762232,0.00016040259,0.0000011373812],"about_ca_topic_score_codex":0.0038235714,"about_ca_topic_score_gemma":0.006768684,"teacher_disagreement_score":0.0038235714,"about_ca_system_score_codex":0.00024775957,"about_ca_system_score_gemma":0.00006586747,"threshold_uncertainty_score":0.007602632},"labels":[],"label_agreement":null},{"id":"W2766289917","doi":"10.3847/1538-4357/aa961d","title":"Seeds Of Life In Space (SOLIS): The Organic Composition Diversity at 300–1000 au Scale in Solar-type Star-forming Regions<sup>*</sup>","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Centre National de la Recherche Scientifique; Science and Technology Facilities Council; Max-Planck-Gesellschaft","keywords":"Organic molecules; Abundance (ecology); Space (punctuation); Scale (ratio); Formamide; Galaxy; Spectral line; Interstellar medium","score_opus":0.013980242652674403,"score_gpt":0.23113610253862704,"score_spread":0.21715585988595265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766289917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978631,0.00011467317,0.00020596788,0.000021318774,0.0000021942465,0.0000025739407,0.00038883992,0.000038390226,0.0013630061],"genre_scores_gemma":[0.9989506,0.00003300972,0.00034367375,0.00000750651,0.000006259041,0.0000019053841,0.0005062504,0.000009862728,0.00014085551],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999542,0.0000036249155,0.0000017685545,0.000017600902,0.000011970661,0.0000107851965],"domain_scores_gemma":[0.99977463,0.00003280991,0.00009560133,0.00001330165,0.000023414575,0.00006033124],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000071950504,0.000191864,0.00011331852,0.001135589,0.00033635198,0.00041226446,0.00017164288,0.0001627932,0.0018296933],"category_scores_gemma":[0.0001572,0.00009273992,0.00014254,0.0005073086,0.00031591332,0.00030962774,0.00036401584,0.00014980612,0.00018936409],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046237954,0.000050901665,0.6057881,0.00009059365,0.00011078762,0.0005895252,0.00075953535,0.0006330722,0.3723895,0.00067925605,0.00093121565,0.017515037],"study_design_scores_gemma":[0.0000039758775,0.000027512051,0.9872602,0.0000029800872,0.000013858369,0.00022155423,0.00024419755,0.0006904893,0.010534877,0.00014432108,0.00085189193,0.000004108859],"about_ca_topic_score_codex":0.0012441588,"about_ca_topic_score_gemma":0.0021100803,"teacher_disagreement_score":0.0018296933,"about_ca_system_score_codex":0.00022906774,"about_ca_system_score_gemma":0.00005541505,"threshold_uncertainty_score":0.00612092},"labels":[],"label_agreement":null},{"id":"W2766452126","doi":"10.3847/1538-4357/aa960c","title":"The Geometry of the Sagittarius Stream from Pan-STARRS1 3π RR Lyrae","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; National Central University; Space Telescope Science Institute; Durham University; Smithsonian Institution; National Science Foundation","keywords":"RR Lyrae variable; Sagittarius; Cepheid variable; Orbital plane; Stars; Plane (geometry); Orbital elements","score_opus":0.011383766621664135,"score_gpt":0.23051465173444463,"score_spread":0.2191308851127805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766452126","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936021,0.0001481228,0.0013489287,0.000039339695,0.0000031712132,0.000007743232,0.0016831663,0.00014438512,0.003022999],"genre_scores_gemma":[0.99573463,0.0001276857,0.001156114,0.000008631423,0.0000059876907,0.0000039348906,0.0025447712,0.00003988059,0.0003783668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999156,0.0000131404495,0.000005110539,0.000025103358,0.000027079961,0.000013987963],"domain_scores_gemma":[0.99977463,0.00001957679,0.00006979018,0.00003314516,0.000061760955,0.000041033556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011004056,0.00017374117,0.0002190171,0.0011495261,0.0002615115,0.00067209813,0.00021661777,0.0001608213,0.0017061017],"category_scores_gemma":[0.00047807323,0.00013775377,0.00022094358,0.0009796647,0.0001735061,0.00026088717,0.0004045229,0.00015499198,0.00075203273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014924996,0.000028447175,0.91874343,0.000052750634,0.000067436406,0.00027156796,0.0005075101,0.018940588,0.018898986,0.0030876128,0.0017693406,0.03748308],"study_design_scores_gemma":[0.000008962768,0.0000324865,0.9722693,0.000011723728,0.000014387546,0.00023159062,0.00018508424,0.01863282,0.0015854914,0.0008291712,0.006182049,0.000016880364],"about_ca_topic_score_codex":0.012015058,"about_ca_topic_score_gemma":0.010734109,"teacher_disagreement_score":0.012015058,"about_ca_system_score_codex":0.0004585987,"about_ca_system_score_gemma":0.00024252495,"threshold_uncertainty_score":0.023890197},"labels":[],"label_agreement":null},{"id":"W2766487124","doi":"10.3847/1538-4357/aa93ec","title":"The Green Bank Ammonia Survey: Observations of Hierarchical Dense Gas Structures in Cepheus-L1251","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; University of Alberta; University of Victoria","funders":"","keywords":"Virial theorem; Centroid; Molecular cloud; Green Bank Telescope; Line (geometry); Kinetic energy; Gravitational collapse","score_opus":0.029616783763051165,"score_gpt":0.27361927100558653,"score_spread":0.24400248724253537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766487124","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998106,0.000038755075,0.00009371276,0.000019710122,0.000001501305,0.0000053306703,0.00081367604,0.000020121597,0.0009011568],"genre_scores_gemma":[0.99846506,0.000026798049,0.00028070074,0.000022766537,0.000004270837,0.000004953818,0.0009508574,0.000004749452,0.00023987953],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990535,0.000011256799,0.0000034466325,0.00002828173,0.000026719463,0.000024904946],"domain_scores_gemma":[0.99973613,0.00002282186,0.00007730106,0.000029601584,0.00004209352,0.00009203501],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012144619,0.00011480675,0.00017318841,0.0008263198,0.00037399397,0.00036084143,0.0002491919,0.00013915,0.0009107275],"category_scores_gemma":[0.0002764701,0.00009759165,0.000100873076,0.00048051498,0.00019083756,0.00012848181,0.00043786567,0.0001219488,0.00030329477],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011672386,0.000047966234,0.96332985,0.000021329164,0.000053986743,0.00031094585,0.00028954886,0.0013845653,0.02089762,0.00019278623,0.0027578664,0.010596804],"study_design_scores_gemma":[0.000005046809,0.00000652544,0.99766445,0.0000036871095,0.0000037178497,0.000026631247,0.000050345003,0.0011923518,0.00054993475,0.00002293796,0.00047109832,0.000003292394],"about_ca_topic_score_codex":0.045965422,"about_ca_topic_score_gemma":0.10222287,"teacher_disagreement_score":0.045965422,"about_ca_system_score_codex":0.0007028388,"about_ca_system_score_gemma":0.00025267844,"threshold_uncertainty_score":0.091395795},"labels":[],"label_agreement":null},{"id":"W2766522901","doi":"10.3847/1538-4357/aaa002","title":"Advanced Diagnostics for the Study of Linearly Polarized Emission. I. Derivation","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Polarization (electrochemistry); Linear polarization; Stokes parameters; Synchrotron radiation; Wavelength; Interferometry; Polarization in astronomy; Elliptical polarization","score_opus":0.0176789693955552,"score_gpt":0.31002435328166084,"score_spread":0.29234538388610565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766522901","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0028856122,0.00076644396,0.99289954,0.00013865363,0.00006782295,0.00003778337,0.00009236306,0.00014504373,0.0029668093],"genre_scores_gemma":[0.24264735,0.0025298162,0.74487317,0.00052431435,0.00031902958,0.00043779096,0.00039575962,0.00024518662,0.008027546],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996593,0.0001052609,0.000023638293,0.00004915314,0.00013367442,0.000028951774],"domain_scores_gemma":[0.9992242,0.00030354163,0.00016114488,0.00008888672,0.00017715748,0.000045126348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087899214,0.0009410667,0.000482435,0.0015862318,0.00033541728,0.0010995294,0.0010180116,0.0010220059,0.001794476],"category_scores_gemma":[0.0026246358,0.00037746967,0.00058904424,0.0010698003,0.0015863887,0.0014776194,0.0013750474,0.0018655244,0.0009916272],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000016248901,0.00003142553,0.0007230238,0.00012929383,0.00001550747,0.0002489638,0.00013554738,0.030143972,0.017095335,0.9129951,0.0019194322,0.036546223],"study_design_scores_gemma":[0.000013898846,0.000057704572,0.0006278344,0.00007137132,0.000010083142,0.0004534211,0.00004616436,0.445632,0.0053452253,0.53027546,0.017420275,0.00004651827],"about_ca_topic_score_codex":0.001070128,"about_ca_topic_score_gemma":0.000680236,"teacher_disagreement_score":0.001794476,"about_ca_system_score_codex":0.0009875016,"about_ca_system_score_gemma":0.0009229915,"threshold_uncertainty_score":0.007164836},"labels":[],"label_agreement":null},{"id":"W2766823892","doi":"10.3847/1538-4357/aa9381","title":"The ISLAnds Project. III. Variable Stars in Six Andromeda Dwarf Spheroidal Galaxies*","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"RR Lyrae variable; Variable star; Milky Way; Andromeda; Local Group; Stars; Globular cluster; Satellite galaxy; Andromeda Galaxy","score_opus":0.012294846570675373,"score_gpt":0.2410463308613565,"score_spread":0.22875148429068112,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766823892","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97026,0.0020202356,0.00038182212,0.00010156877,0.0000092335895,0.00007057181,0.021281432,0.000077817866,0.0057973093],"genre_scores_gemma":[0.9503378,0.0010902889,0.003124719,0.000057602534,0.000022455844,0.000097376724,0.04126939,0.000076416196,0.00392402],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995714,0.000088892084,0.00002887134,0.00012804232,0.00010682636,0.00007595386],"domain_scores_gemma":[0.99931514,0.000067390545,0.00014870605,0.00011484704,0.0001479799,0.00020599712],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005084402,0.00037214087,0.00035120736,0.0031666353,0.00035617722,0.0007697414,0.00039897987,0.00019315165,0.0024356851],"category_scores_gemma":[0.00087980274,0.00014458362,0.00027150332,0.0018249812,0.00021521293,0.00026750067,0.0012178777,0.00016095386,0.0008713731],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005754196,0.000058558304,0.9343049,0.00021372642,0.00019209119,0.000195482,0.0011724782,0.0002888772,0.0027211516,0.00072764,0.0040519745,0.055497732],"study_design_scores_gemma":[0.000026868338,0.00004792248,0.9809585,0.000052905005,0.00007422464,0.00031750664,0.0005472666,0.00030632052,0.00055331696,0.0000939188,0.017010847,0.000010410403],"about_ca_topic_score_codex":0.046627864,"about_ca_topic_score_gemma":0.070151515,"teacher_disagreement_score":0.046627864,"about_ca_system_score_codex":0.00047449998,"about_ca_system_score_gemma":0.00051161717,"threshold_uncertainty_score":0.09271294},"labels":[],"label_agreement":null},{"id":"W2766857360","doi":"10.3847/1538-4357/aab2b0","title":"Can We Distinguish Low-mass Black Holes in Neutron Star Binaries?","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Physics; LIGO; Neutron star; Gravitational wave; Astrophysics; Binary number; Black hole (networking); Binary black hole; Mass ratio; Astronomy; Equation of state; Quantum mechanics","score_opus":0.012207593888306474,"score_gpt":0.3008388397392061,"score_spread":0.2886312458508996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766857360","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9623686,0.020687228,0.0056172768,0.0032117611,0.00036917854,0.000019697136,0.00023071183,0.000037785998,0.0074576507],"genre_scores_gemma":[0.9956084,0.0017983352,0.0015260548,0.00041788988,0.00016869565,0.0000038192866,0.0001245782,0.00000565742,0.00034651454],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99970704,0.00009348332,0.000027661543,0.000056617668,0.000060284547,0.000054876673],"domain_scores_gemma":[0.998692,0.00057895505,0.00033999895,0.000071577364,0.00011934027,0.00019823606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015748903,0.00028124973,0.0004936695,0.0012964556,0.00037994268,0.001669022,0.00046071855,0.00087905617,0.0017646555],"category_scores_gemma":[0.004914758,0.0001403679,0.0002020959,0.0006439338,0.0010602913,0.0019980539,0.00080211414,0.00065321015,0.00049567013],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018233702,0.00013210787,0.8463416,0.0004883032,0.00015848667,0.0011976587,0.00064578897,0.001021147,0.011951103,0.015517656,0.0023868198,0.11833595],"study_design_scores_gemma":[0.00008870863,0.000383292,0.8440633,0.0007438371,0.00013731982,0.004886731,0.0026538204,0.010279616,0.008187895,0.110172875,0.018309707,0.000092786846],"about_ca_topic_score_codex":0.0009910299,"about_ca_topic_score_gemma":0.0016479715,"teacher_disagreement_score":0.0017646555,"about_ca_system_score_codex":0.00030027464,"about_ca_system_score_gemma":0.00019675533,"threshold_uncertainty_score":0.008328915},"labels":[],"label_agreement":null},{"id":"W2766873047","doi":"10.3847/1538-4357/aa951c","title":"The Survey of Water and Ammonia in the Galactic Center (SWAG): Molecular Cloud Evolution in the Central Molecular Zone","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Galactic Center; Mean kinetic temperature; Milky Way; Molecular cloud; Kinetic energy; Star formation; Line (geometry); Metallicity","score_opus":0.009139518422351826,"score_gpt":0.2401777066510533,"score_spread":0.23103818822870148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2766873047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99964035,0.00005292841,0.000030835232,0.000008570552,5.163339e-7,0.0000012102788,0.000090014684,0.0000029041637,0.00017264148],"genre_scores_gemma":[0.99953234,0.00003577409,0.0001083618,0.0000069283687,0.0000023279104,0.0000013537721,0.000224512,0.0000013739766,0.000086932836],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992263,0.000008464807,0.0000035134283,0.000021305988,0.000019785713,0.000024300525],"domain_scores_gemma":[0.9998011,0.000014959224,0.00006265336,0.000011682231,0.000041986725,0.00006762804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013182245,0.00014257318,0.00014910525,0.00072741276,0.00024230192,0.00027014696,0.00020769032,0.00016946149,0.0004491371],"category_scores_gemma":[0.00021418817,0.00008566654,0.000116772484,0.000578181,0.00017757031,0.00019953688,0.00032491068,0.00011580632,0.00010791951],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007537616,0.000029221676,0.9699505,0.000011539175,0.000047465805,0.000084954205,0.0001878706,0.00015222831,0.02497947,0.00006456593,0.00013046844,0.0042863716],"study_design_scores_gemma":[0.000001912769,0.000013804746,0.99895275,0.0000014204899,0.0000046899754,0.00003416704,0.000058617512,0.00018920016,0.00055136107,0.0000066137236,0.00018465913,8.6654285e-7],"about_ca_topic_score_codex":0.01846948,"about_ca_topic_score_gemma":0.03345011,"teacher_disagreement_score":0.01846948,"about_ca_system_score_codex":0.00028947808,"about_ca_system_score_gemma":0.00016284554,"threshold_uncertainty_score":0.03672397},"labels":[],"label_agreement":null},{"id":"W2767158222","doi":"10.3847/1538-4357/aaa765","title":"Stellar Multiplicity Meets Stellar Evolution and Metallicity: The APOGEE View","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Stars; Milky Way; Red-giant branch; Stellar evolution; Circumbinary planet; Stellar collision; Red clump; Stellar kinematics; Binary star; Main sequence","score_opus":0.013890118590014875,"score_gpt":0.23337526233398123,"score_spread":0.21948514374396635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767158222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9833491,0.00300078,0.0046795746,0.0018870821,0.000036432,0.0000036871415,0.00037973444,0.00004867187,0.006614982],"genre_scores_gemma":[0.99880433,0.00030805584,0.00030295728,0.000099762365,0.00008589587,0.0000010632243,0.00006678524,0.0000066571665,0.00032459668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977833,0.000063069405,0.000013404377,0.000083245905,0.000040877123,0.00002111618],"domain_scores_gemma":[0.9975284,0.0012259192,0.0005305368,0.00022669116,0.00015008326,0.00033849795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078584265,0.00032925248,0.00054209295,0.0013141325,0.00031295072,0.0016735347,0.00037738672,0.0004888894,0.0028840085],"category_scores_gemma":[0.0027918625,0.0001479098,0.00025095028,0.00075096136,0.0010597884,0.0016909111,0.0010626819,0.0007212376,0.00032901025],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022446128,0.00002904968,0.96495163,0.00005065214,0.00017503901,0.0002757645,0.00023022271,0.001512366,0.0036914814,0.0052535525,0.0008931494,0.02271276],"study_design_scores_gemma":[0.000013952539,0.00014014784,0.97458386,0.00003364517,0.000076431774,0.0008095699,0.0005277594,0.0071491185,0.0007641921,0.012817621,0.0030603998,0.00002321755],"about_ca_topic_score_codex":0.0015464571,"about_ca_topic_score_gemma":0.001428237,"teacher_disagreement_score":0.0028840085,"about_ca_system_score_codex":0.00026331464,"about_ca_system_score_gemma":0.00018028068,"threshold_uncertainty_score":0.009647965},"labels":[],"label_agreement":null},{"id":"W2767230474","doi":"10.3847/1538-4357/aab36e","title":"Jets in Hydrogen-poor Superluminous Supernovae: Constraints from a Comprehensive Analysis of Radio Observations","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Agence Nationale de la Recherche","keywords":"Ejecta; Astrophysical jet; Luminosity; Supernova; Collimated light; Jet (fluid); Merlin (protein); Energy (signal processing)","score_opus":0.026132449545070303,"score_gpt":0.25098183465651436,"score_spread":0.22484938511144406,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767230474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993001,0.00095188216,0.0026481033,0.000019425952,0.0000040779473,0.000016012134,0.0019186272,0.00012745081,0.001313511],"genre_scores_gemma":[0.9889726,0.0007328768,0.0031600068,0.00003156039,0.000026683125,0.00002022251,0.006747371,0.00005006098,0.00025863416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997863,0.000031017804,0.00002843871,0.000056559555,0.000057267316,0.00004042534],"domain_scores_gemma":[0.998643,0.00046886556,0.00045507628,0.00016611593,0.00011244084,0.00015440899],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063657906,0.00042098638,0.00038104644,0.0026666145,0.00019898609,0.0010877858,0.00027190277,0.00017368403,0.00065581163],"category_scores_gemma":[0.0010464845,0.00019699991,0.0005412413,0.001659729,0.00017577775,0.00032308517,0.0006176976,0.00014824205,0.0002622833],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019504596,0.000054601423,0.94630814,0.00010309624,0.00028257625,0.00042086717,0.0001605998,0.0024098817,0.023266874,0.00018496103,0.00039354758,0.026219716],"study_design_scores_gemma":[0.0000063265593,0.000041369556,0.9941917,0.000018451654,0.00009844566,0.0001874706,0.000073905576,0.0021930581,0.0016235451,0.00016103836,0.0013956408,0.000008992909],"about_ca_topic_score_codex":0.001577715,"about_ca_topic_score_gemma":0.0024426025,"teacher_disagreement_score":0.0026666145,"about_ca_system_score_codex":0.00011906332,"about_ca_system_score_gemma":0.00013898556,"threshold_uncertainty_score":0.0033665895},"labels":[],"label_agreement":null},{"id":"W2767253059","doi":"10.3847/1538-4357/aa9923","title":"Testing for Shock-heated X-Ray Gas around Compact Steep Spectrum Radio Galaxies","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Office of Naval Research; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; National Radio Astronomy Observatory; Ohio State University; University of Notre Dame; Smithsonian Institution; Alfred P. Sloan Foundation; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; University of Minnesota; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Physics; Astrophysics; Radio galaxy; X-shaped radio galaxy; Galaxy; Astronomy; Active galactic nucleus; Redshift; Galaxy cluster","score_opus":0.01886956765159512,"score_gpt":0.24326840114644122,"score_spread":0.2243988334948461,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767253059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987739,0.000078458885,0.00025810336,0.000015272917,0.0000032076298,0.0000065829604,0.00008233132,0.00001966792,0.00076251937],"genre_scores_gemma":[0.99968016,0.000015157039,0.00011906426,0.000010606517,0.0000037924053,0.0000021933295,0.00007170526,0.0000018982988,0.000095316194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997869,0.000026884372,0.00001704394,0.00003952602,0.00005134088,0.000078258396],"domain_scores_gemma":[0.99843603,0.00038514117,0.00046217247,0.00012361778,0.00017706705,0.0004159372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041348478,0.0003123638,0.00019015695,0.00089088187,0.00035796574,0.0007839735,0.00065382454,0.00026874457,0.002466469],"category_scores_gemma":[0.0010079277,0.00014131967,0.0003253229,0.00040550478,0.0005515689,0.00032009862,0.0005779441,0.0002580389,0.00035725525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019947626,0.000039241197,0.9766144,0.000020922991,0.000044597247,0.0005067949,0.00016721361,0.0002102319,0.019213023,0.00020283001,0.00008030942,0.002701029],"study_design_scores_gemma":[0.000008571294,0.00018641568,0.99275804,0.000009630112,0.000026274074,0.00044022937,0.00041804917,0.0006700582,0.005026333,0.00007942797,0.00037167722,0.0000053350777],"about_ca_topic_score_codex":0.0019684357,"about_ca_topic_score_gemma":0.0015518633,"teacher_disagreement_score":0.002466469,"about_ca_system_score_codex":0.00022296522,"about_ca_system_score_gemma":0.00012336587,"threshold_uncertainty_score":0.00825119},"labels":[],"label_agreement":null},{"id":"W2767340572","doi":"10.3847/1538-4357/aa9703","title":"The Green Bank Ammonia Survey: Unveiling the Dynamics of the Barnard 59 Star-forming Clump","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Alberta; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Star formation; Gravitational collapse; Virial theorem; Thermal; Gravitation; Turbulence; Stars; Magnetic field; Line (geometry)","score_opus":0.015029719907192093,"score_gpt":0.2535725519361613,"score_spread":0.2385428320289692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767340572","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998855,0.000060993003,0.000043951473,0.00003862234,0.0000022587017,0.000004215032,0.000329429,0.0000043036544,0.0006611658],"genre_scores_gemma":[0.9988393,0.00007952367,0.000207582,0.000045692475,0.000007208072,0.0000032547755,0.00048569837,0.0000044658427,0.00032730785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999244,0.000010782777,0.00000317121,0.00002048836,0.000019650017,0.000021436055],"domain_scores_gemma":[0.9997565,0.000021851882,0.000071581264,0.000012249136,0.00004004652,0.00009772417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019582774,0.0001261916,0.00022487088,0.00090355956,0.00036932706,0.00036218812,0.0002573085,0.00019707113,0.0011967779],"category_scores_gemma":[0.00025859548,0.00009637222,0.00006579446,0.00051298225,0.00028172313,0.00021436591,0.0006055434,0.00023072682,0.00039854177],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000091990834,0.000043743905,0.9846399,0.00001353888,0.000018885457,0.0003383773,0.0003365655,0.0001028763,0.009520803,0.00013130551,0.0005732045,0.0041889013],"study_design_scores_gemma":[0.0000048211273,0.000024962674,0.99800926,0.000007999807,0.0000055940613,0.00007789681,0.00031119466,0.0003631528,0.00033598812,0.000029649253,0.0008269049,0.0000025733552],"about_ca_topic_score_codex":0.03238052,"about_ca_topic_score_gemma":0.07148749,"teacher_disagreement_score":0.03238052,"about_ca_system_score_codex":0.00035111027,"about_ca_system_score_gemma":0.00027965076,"threshold_uncertainty_score":0.0643841},"labels":[],"label_agreement":null},{"id":"W2767610311","doi":"10.3847/1538-4357/aa98dc","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Hα and Hβ Reverberation Measurements from First-year Spectroscopy and Photometry","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":222,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; York University","funders":"Science and Technology Facilities Council","keywords":"Reverberation mapping; Sky; Photometry (optics); Reverberation; Light curve; Redshift; Emission spectrum; Spectroscopy","score_opus":0.023844698307836525,"score_gpt":0.24546140014068962,"score_spread":0.2216167018328531,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767610311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9781455,0.00026213523,0.0039345436,0.00005832184,0.000028426368,0.00006456046,0.013634304,0.0008778593,0.0029943408],"genre_scores_gemma":[0.94848865,0.00017187948,0.014011449,0.000053434305,0.000048832382,0.00009856946,0.03485355,0.00029591925,0.0019777117],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99915373,0.00012558898,0.000049750644,0.00016626035,0.00034687176,0.00015774275],"domain_scores_gemma":[0.99756527,0.00012450895,0.0006321603,0.00058392,0.000754567,0.0003395652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016282666,0.0007092272,0.00038383954,0.00261372,0.00042447372,0.00065523223,0.00048896956,0.00026368746,0.0016394655],"category_scores_gemma":[0.0016308826,0.00030565562,0.00043262096,0.0014436013,0.0001961428,0.00048539334,0.0010884969,0.00039876922,0.0013499549],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004802858,0.00023952477,0.885969,0.00016851339,0.00039740573,0.00032969902,0.0008452615,0.0030827022,0.02354864,0.00020850799,0.009760177,0.07497025],"study_design_scores_gemma":[0.0000122439415,0.00005855525,0.98871255,0.000008865883,0.000028616694,0.00011349066,0.00009626712,0.0015849387,0.0047383797,0.000034176024,0.004597508,0.00001432624],"about_ca_topic_score_codex":0.016035564,"about_ca_topic_score_gemma":0.029418623,"teacher_disagreement_score":0.016035564,"about_ca_system_score_codex":0.00039157097,"about_ca_system_score_gemma":0.00040279672,"threshold_uncertainty_score":0.03188443},"labels":[],"label_agreement":null},{"id":"W2767651365","doi":"10.3847/1538-4357/aabd80","title":"SILVERRUSH. V. Census of Lyα, [O iii] λ5007, Hα, and [C ii] 158 μm Line Emission with ∼1000 LAEs at z = 4.9–7.0 Revealed with Subaru/HSC","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; National Research Foundation; High Energy Accelerator Research Organization; National Central University; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; Eötvös Loránd Tudományegyetem; Academia Sinica; Space Telescope Science Institute; Princeton University; Johns Hopkins University; National Astronomical Observatory of Japan; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; Japan Society for the Promotion of Science; Queen's University Belfast; Durham University; Japan Science and Technology Agency; Smithsonian Institution; National Science Foundation","keywords":"Equivalent width; Galaxy; Luminosity; Flux (metallurgy); Emission spectrum; Line (geometry); Star formation; Quasar","score_opus":0.006233617794497272,"score_gpt":0.20708780235279464,"score_spread":0.20085418455829737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767651365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997493,0.00009601352,0.00005709494,0.000020279369,0.0000014871375,0.0000024110325,0.0014363123,0.000019149615,0.00087427394],"genre_scores_gemma":[0.99437153,0.000054811433,0.00013416405,0.000016970174,0.000007512637,0.000004059223,0.00483593,0.0000062086,0.0005688518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998772,0.000014698129,0.00000809561,0.000028988035,0.00003654091,0.00003440298],"domain_scores_gemma":[0.9995554,0.000034947796,0.0001493593,0.00005038869,0.00008706186,0.00012286159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017737149,0.0001420617,0.00013520637,0.0015239649,0.00015816603,0.00029840393,0.00017604293,0.000105130704,0.0011436151],"category_scores_gemma":[0.00031989912,0.00007584695,0.00015653035,0.0006505827,0.000121066834,0.000195535,0.00032835442,0.00010780729,0.0004911558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010733066,0.000021164431,0.98323244,0.000013727244,0.00003010523,0.00009635483,0.000116149226,0.00010304254,0.006796059,0.000106930565,0.0009365972,0.008440106],"study_design_scores_gemma":[0.0000011344011,0.000012512227,0.9988952,0.0000011182901,0.0000041950257,0.00004271885,0.00003512194,0.000121413206,0.0003826949,0.0000075468856,0.0004955334,8.006263e-7],"about_ca_topic_score_codex":0.0075694784,"about_ca_topic_score_gemma":0.007312297,"teacher_disagreement_score":0.0075694784,"about_ca_system_score_codex":0.00021423413,"about_ca_system_score_gemma":0.00014827696,"threshold_uncertainty_score":0.015050888},"labels":[],"label_agreement":null},{"id":"W2767675395","doi":"10.3847/1538-4357/ab0f36","title":"Intensity-coupled Polarization in Instruments with a Continuously Rotating Half-wave Plate","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; McGill University","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Polarization (electrochemistry); Physics; Cosmic microwave background; Linearity; Optics; Waveplate; Detector; Linear polarization; Brewster's angle; Radial polarization; Chemistry; Laser beams","score_opus":0.0058151625021458705,"score_gpt":0.21022434934532996,"score_spread":0.2044091868431841,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767675395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8216259,0.000512763,0.17161873,0.00017889873,0.00007567467,0.00007780413,0.00036828383,0.0007729173,0.0047690524],"genre_scores_gemma":[0.91253865,0.00029116496,0.08532658,0.000116133415,0.000050217983,0.00007490419,0.00034027785,0.00016201848,0.0010999686],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986985,0.0003423794,0.000052651998,0.00025099493,0.0005237728,0.00013174572],"domain_scores_gemma":[0.997154,0.0010382662,0.000597126,0.00067993527,0.00046463037,0.000065997025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001412748,0.00054444594,0.00031627645,0.00076104695,0.00030363415,0.00072842726,0.00079478155,0.00049896876,0.001671432],"category_scores_gemma":[0.003232351,0.00048793922,0.00032696401,0.0018122094,0.0008472593,0.0010986468,0.0009803687,0.0006145911,0.00045639486],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012131804,0.00017631278,0.07347436,0.00030904546,0.0002753703,0.0003656911,0.0003106866,0.015099398,0.75999385,0.0052021407,0.0006496954,0.14293021],"study_design_scores_gemma":[0.000048894548,0.00034630566,0.08950033,0.00003863269,0.00016253836,0.0004914674,0.00010499832,0.050305784,0.8530608,0.0017723832,0.0040761977,0.00009172293],"about_ca_topic_score_codex":0.0007315097,"about_ca_topic_score_gemma":0.0010051749,"teacher_disagreement_score":0.001671432,"about_ca_system_score_codex":0.0003771159,"about_ca_system_score_gemma":0.000278358,"threshold_uncertainty_score":0.007471442},"labels":[],"label_agreement":null},{"id":"W2767899068","doi":"10.3847/1538-4357/aae37c","title":"Stripping of the Hot Gas Halos in Member Galaxies of Abell 1795","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Intracluster medium; Cluster (spacecraft); Surface brightness; Halo; Galaxy cluster; Ram pressure; RADIUS; Galaxy","score_opus":0.010618774506200246,"score_gpt":0.22120627583032035,"score_spread":0.2105875013241201,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2767899068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991548,0.000020249268,0.00017184798,0.000005292478,8.8957455e-7,0.0000020944944,0.0001331677,0.000018077337,0.00049358833],"genre_scores_gemma":[0.9992912,0.000009425645,0.00024180963,0.000004727522,0.0000013999085,0.0000016171701,0.0002663041,0.0000057705797,0.00017770764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999931,0.000005546931,0.0000033761087,0.00002169784,0.000019839503,0.000018681085],"domain_scores_gemma":[0.9997849,0.000023415978,0.000057370056,0.000037505873,0.000020332905,0.00007651511],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001479204,0.00012689436,0.00020344928,0.0006359481,0.0004378926,0.00039699848,0.00020623146,0.00013409689,0.0010911438],"category_scores_gemma":[0.00029812267,0.00008482495,0.00021326279,0.0004783467,0.00024240611,0.00015623719,0.00038911574,0.00011097864,0.00024682423],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005455125,0.000115020055,0.80440587,0.00006318876,0.0001104461,0.00064434286,0.00094599195,0.0054636346,0.16758047,0.00143719,0.0008426478,0.017845688],"study_design_scores_gemma":[0.0000031306158,0.000034856716,0.99193734,0.000002894543,0.000008421797,0.00007657541,0.00012816192,0.0023390625,0.004776784,0.00011072086,0.00057655905,0.000005451925],"about_ca_topic_score_codex":0.011178559,"about_ca_topic_score_gemma":0.010742721,"teacher_disagreement_score":0.011178559,"about_ca_system_score_codex":0.00053380756,"about_ca_system_score_gemma":0.00019960786,"threshold_uncertainty_score":0.02222699},"labels":[],"label_agreement":null},{"id":"W2768013095","doi":"10.3847/1538-4357/aacbd2","title":"The Effect of Massive Neutrinos on the Position of Cold Dark Matter Halo: Revealed via the Delaunay Triangulation Void","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Natural Science Foundation of China-Guangdong Joint Fund; National Natural Science Foundation of China; Fundamental Research Funds for the Central Universities; National Science Foundation","keywords":"Halo; Void (composites); Neutrino; Dark matter; Cold dark matter; Galaxy; Delaunay triangulation","score_opus":0.003916865643868771,"score_gpt":0.20558592562909822,"score_spread":0.20166905998522944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2768013095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9800009,0.000091619266,0.017568612,0.00013268339,0.000020293453,0.000015696229,0.00023283552,0.00018309294,0.0017541472],"genre_scores_gemma":[0.99163204,0.0000241855,0.0079294015,0.000018323448,0.0000037031768,0.000008830339,0.00016596464,0.000037716683,0.00017986572],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99978405,0.00008743561,0.0000071165264,0.000038488386,0.00003887773,0.000044039407],"domain_scores_gemma":[0.9984428,0.000890122,0.0001926629,0.00015133842,0.00014154345,0.00018150118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005505332,0.00029805192,0.00037081004,0.00053971825,0.0005089561,0.00064206746,0.00071610336,0.0005208766,0.0013633682],"category_scores_gemma":[0.003664997,0.00026019264,0.0004455056,0.00043234558,0.0007234011,0.000532052,0.001128939,0.00041840662,0.0001062882],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018606977,0.000047722457,0.02733741,0.00003525864,0.00006563872,0.00014893478,0.00015074585,0.9611736,0.0028948393,0.003841168,0.00038184482,0.0037367162],"study_design_scores_gemma":[0.000012659536,0.000017362976,0.001859546,0.0000037941284,0.000005134797,0.00001559807,0.00004187601,0.9965193,0.00046166262,0.000923833,0.00013103244,0.00000819123],"about_ca_topic_score_codex":0.015600503,"about_ca_topic_score_gemma":0.009369034,"teacher_disagreement_score":0.015600503,"about_ca_system_score_codex":0.00056866644,"about_ca_system_score_gemma":0.00062048674,"threshold_uncertainty_score":0.03101939},"labels":[],"label_agreement":null},{"id":"W2769478074","doi":"10.3847/1538-4357/aa9d19","title":"To the Galactic Virial Radius with Hyper Suprime-Cam","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; National Central University; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; Eötvös Loránd Tudományegyetem; European Commission; Academia Sinica; Space Telescope Science Institute; Los Alamos National Laboratory; Princeton University; Johns Hopkins University; Japan Society for the Promotion of Science; Queen's University Belfast; National Aeronautics and Space Administration; Durham University; Japan Science and Technology Agency; Smithsonian Institution; National Science Foundation","keywords":"Stars; Galaxy; Galactic halo; Halo; Milky Way; Stellar density; Photometry (optics); RADIUS; Star count","score_opus":0.00985139069655173,"score_gpt":0.22092715374020203,"score_spread":0.2110757630436503,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2769478074","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95570046,0.0006984418,0.015197245,0.00039271696,0.000060891147,0.00002431646,0.0032316819,0.0019416043,0.022752743],"genre_scores_gemma":[0.9901516,0.000060659702,0.0076951487,0.000060416933,0.000036747613,0.000011026187,0.0014316913,0.00006311186,0.0004896545],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997731,0.00005367166,0.0000082290335,0.000073177944,0.000059513564,0.00003234851],"domain_scores_gemma":[0.99907756,0.0002088698,0.00023146781,0.00028276903,0.00010071543,0.0000985652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005847884,0.0002753088,0.00017182005,0.0010688697,0.0001659136,0.0007210696,0.00046744655,0.00019223317,0.0028694689],"category_scores_gemma":[0.002316098,0.00015565964,0.00024139315,0.0006925176,0.0003337904,0.0005845468,0.0006725037,0.00032235688,0.0005545156],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068455,0.00008618631,0.74861056,0.0001404815,0.00021250239,0.00037355558,0.00032042534,0.03407064,0.035353307,0.013911583,0.010371189,0.15586497],"study_design_scores_gemma":[0.000026216061,0.00010946405,0.8170413,0.0000432851,0.000042790198,0.00035896536,0.00012106702,0.15197338,0.0114825005,0.0070998357,0.011672264,0.000028897404],"about_ca_topic_score_codex":0.0018340102,"about_ca_topic_score_gemma":0.002483213,"teacher_disagreement_score":0.0028694689,"about_ca_system_score_codex":0.00032278098,"about_ca_system_score_gemma":0.00017097824,"threshold_uncertainty_score":0.009599268},"labels":[],"label_agreement":null},{"id":"W2770242612","doi":"10.3847/1538-4357/aab498","title":"The Stellar Populations of Two Ultra-diffuse Galaxies from Optical and Near-infrared Photometry","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Virgo Cluster; Galaxy; Surface brightness; Photometry (optics); Metallicity; Surface brightness fluctuation; Stellar population; Star formation; Stellar mass","score_opus":0.011335077927415914,"score_gpt":0.24032156272702512,"score_spread":0.2289864847996092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2770242612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985663,0.00006652658,0.00043356957,0.000008165816,8.719047e-7,0.0000017091787,0.00021121529,0.000012761913,0.0006988782],"genre_scores_gemma":[0.99905306,0.0000177452,0.00030608094,0.000005731628,0.0000015352762,0.0000011556491,0.00053583167,0.0000021619503,0.00007670267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998622,0.000014514943,0.000005176588,0.000050526887,0.000035334997,0.000032351854],"domain_scores_gemma":[0.9992824,0.00011469836,0.00018905713,0.00013598276,0.0001195934,0.00015821838],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029769778,0.00021965976,0.00018510957,0.0010986788,0.00017509943,0.00056703296,0.00040342097,0.00019368518,0.0008402454],"category_scores_gemma":[0.0006503958,0.00012649568,0.00016746215,0.00054440263,0.0003273046,0.00024825352,0.00054581714,0.00015600615,0.00021487646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012040898,0.0000193744,0.98225963,0.00001931588,0.000035515317,0.00004014894,0.000134742,0.00070763566,0.0072063077,0.0004914598,0.00018655161,0.008778917],"study_design_scores_gemma":[0.000007099479,0.00003649339,0.9928831,0.0000124126755,0.00002645763,0.00010837959,0.00019504697,0.0032240078,0.0021530394,0.00037993095,0.0009678445,0.000006149363],"about_ca_topic_score_codex":0.004252196,"about_ca_topic_score_gemma":0.008157209,"teacher_disagreement_score":0.004252196,"about_ca_system_score_codex":0.00036359148,"about_ca_system_score_gemma":0.000105827436,"threshold_uncertainty_score":0.008454919},"labels":[],"label_agreement":null},{"id":"W2770365887","doi":"10.3847/1538-4357/aaa12a","title":"A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray-luminous Classical Nova to Date","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Ejecta; Physics; Astrophysics; Nova (rocket); Light curve; Brightness; Gamma ray; Astronomy; Gamma-ray burst; Supernova","score_opus":0.03720563713179829,"score_gpt":0.2783651864210227,"score_spread":0.24115954928922442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2770365887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983797,0.00006772093,0.00007613473,0.000006057329,0.0000012249152,0.0000074628515,0.000742013,0.0000073565598,0.0007123831],"genre_scores_gemma":[0.99642533,0.00005688564,0.00028130252,0.000009375482,0.000005220212,0.000008379964,0.0029353013,0.000008063069,0.0002701385],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980754,0.000016795671,0.000014534317,0.000051245177,0.000053974873,0.000055908204],"domain_scores_gemma":[0.99927074,0.000077898265,0.00021230064,0.00008041226,0.00009821031,0.00026053525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023429816,0.0003603332,0.00031815574,0.0025326107,0.000698075,0.00042169166,0.000255302,0.00018296053,0.00085886876],"category_scores_gemma":[0.0005364594,0.0001524402,0.00027337478,0.0014898941,0.00027989136,0.0002116917,0.00069332425,0.0001823447,0.00022843239],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001312654,0.00004940894,0.97484946,0.000041116356,0.000062971674,0.00046811334,0.00020686525,0.0004255133,0.016640425,0.00011145833,0.00040840864,0.0066050263],"study_design_scores_gemma":[0.0000016821991,0.000024256295,0.9987149,0.0000038444937,0.0000055477035,0.0001900034,0.000060475828,0.00014175712,0.0002894955,0.000021035179,0.0005447156,0.0000023442071],"about_ca_topic_score_codex":0.012863154,"about_ca_topic_score_gemma":0.033692583,"teacher_disagreement_score":0.012863154,"about_ca_system_score_codex":0.00045552276,"about_ca_system_score_gemma":0.00027454784,"threshold_uncertainty_score":0.025576591},"labels":[],"label_agreement":null},{"id":"W2771606251","doi":"10.3847/1538-4357/aa9e86","title":"Banyan. X. Discovery of a Wide, Low-gravity L-type Companion to a Fast-rotating M3 Dwarf<sup>*</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Stars; Astrophysics; Physics; Astrometry; Astronomy; Outlier; Type (biology); Geology; Paleontology; Computer science; Artificial intelligence","score_opus":0.011454764754696367,"score_gpt":0.24048576722932047,"score_spread":0.2290310024746241,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2771606251","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.960131,0.001993072,0.0019890903,0.00074227416,0.00013505323,0.000035575697,0.0011225281,0.00020017294,0.03365126],"genre_scores_gemma":[0.9826057,0.0008388555,0.0033079642,0.00047120915,0.00008279269,0.00002205386,0.002500942,0.000038164428,0.010132308],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992347,0.0000045977604,0.0000043526406,0.00003513135,0.000018877516,0.000013502582],"domain_scores_gemma":[0.99980944,0.000022581804,0.00005837294,0.000027333237,0.000023520784,0.000058752605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015519769,0.00021502814,0.00012507438,0.0005034512,0.0010726424,0.00070943,0.00044971996,0.0005818035,0.0051756552],"category_scores_gemma":[0.00023723165,0.00011651867,0.00013378283,0.0006423836,0.0003226099,0.000342031,0.00072921935,0.00033381395,0.0023077554],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012092947,0.0001418418,0.33160755,0.00050172023,0.00006237465,0.03131622,0.00078037544,0.00023723375,0.48537523,0.007839489,0.005897789,0.13503087],"study_design_scores_gemma":[0.000048466896,0.00030789388,0.69426566,0.000092679285,0.000090694404,0.05895185,0.0007731863,0.0011652797,0.110132046,0.0051875594,0.12894507,0.00003959769],"about_ca_topic_score_codex":0.0025537773,"about_ca_topic_score_gemma":0.0021025834,"teacher_disagreement_score":0.0051756552,"about_ca_system_score_codex":0.00027454313,"about_ca_system_score_gemma":0.0002598914,"threshold_uncertainty_score":0.017314255},"labels":[],"label_agreement":null},{"id":"W2771677172","doi":"10.3847/1538-4357/aaaf6f","title":"Parameterizing the Supernova Engine and Its Effect on Remnants and Basic Yields","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Los Alamos National Laboratory; Laboratory Directed Research and Development; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; National Science Foundation","keywords":"Supernova; Supernova remnant; Range (aeronautics); Convection; Explosive material; Mass distribution","score_opus":0.012903562490582091,"score_gpt":0.2377581482502582,"score_spread":0.22485458575967612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2771677172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911137,0.00016793938,0.00681134,0.00006492384,0.000010550846,0.000015527728,0.00028870197,0.00009212776,0.0014352737],"genre_scores_gemma":[0.9989593,0.000049062823,0.00062652596,0.000011994855,0.000002663652,0.000011220758,0.0001962758,0.00002222787,0.000120750665],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993838,0.00028749093,0.000040153107,0.00014736656,0.00005761109,0.00008355842],"domain_scores_gemma":[0.9927713,0.0053244676,0.0005450876,0.0009905861,0.00014252668,0.00022600376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023878329,0.0013698838,0.00047178983,0.0008422851,0.00034159937,0.0014560263,0.0010059706,0.00076360913,0.0018620649],"category_scores_gemma":[0.0076437974,0.0004753615,0.001125177,0.0006691814,0.0011903787,0.0011581426,0.0013663546,0.0007994164,0.00025079123],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013319084,0.00028414303,0.11815964,0.00012174296,0.00084255025,0.0004044468,0.000119997676,0.82877296,0.03436537,0.0068954728,0.00029028018,0.008411468],"study_design_scores_gemma":[0.00031403045,0.0010912361,0.120628834,0.00011513769,0.0011629271,0.00047129169,0.00034470047,0.7357578,0.1193818,0.017604077,0.0028182147,0.0003099149],"about_ca_topic_score_codex":0.0022052242,"about_ca_topic_score_gemma":0.0008901415,"teacher_disagreement_score":0.0023878329,"about_ca_system_score_codex":0.00049676036,"about_ca_system_score_gemma":0.00028618702,"threshold_uncertainty_score":0.012628257},"labels":[],"label_agreement":null},{"id":"W2772226354","doi":"10.3847/1538-4357/aaa0d0","title":"Computing the Polarimetric and Photometric Variability of Be Stars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Red Deer Polytechnic; Western University","funders":"","keywords":"Polarization (electrochemistry); Position angle; Radiative transfer; Polarimetry; Observable; Monte Carlo method; Linear polarization; Stars","score_opus":0.013308810754571673,"score_gpt":0.25714478616204506,"score_spread":0.24383597540747337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2772226354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99347717,0.00003156864,0.005421622,0.000017881093,0.0000026751352,0.0000057970415,0.0003512124,0.00018794627,0.00050418265],"genre_scores_gemma":[0.9967604,0.000013636491,0.002284616,0.0000048513,0.0000038114406,0.0000026339715,0.00082434755,0.00001670069,0.00008902588],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999798,0.000031116768,0.000007970881,0.00009477891,0.000035824884,0.000032291307],"domain_scores_gemma":[0.9993861,0.00023097383,0.000113806724,0.00008121711,0.000097889206,0.00009001428],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000365065,0.00032349446,0.0003173974,0.0012453912,0.00022980955,0.00085234613,0.0003517,0.00044392142,0.00068136136],"category_scores_gemma":[0.002023893,0.00025634692,0.00043186528,0.0007289435,0.00022228704,0.00047818988,0.00033993946,0.00023531164,0.00033137528],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057556404,0.00013607694,0.63306534,0.000043930384,0.0002104859,0.00019992708,0.00014660257,0.31016275,0.021822596,0.0007775738,0.0005647407,0.03229445],"study_design_scores_gemma":[0.000015425558,0.00006681541,0.23867446,0.000004476025,0.000026276872,0.0001107597,0.0000877004,0.7545497,0.0051556556,0.00084608555,0.00044280145,0.000019941737],"about_ca_topic_score_codex":0.0041025877,"about_ca_topic_score_gemma":0.002652319,"teacher_disagreement_score":0.0041025877,"about_ca_system_score_codex":0.0003757125,"about_ca_system_score_gemma":0.00016853413,"threshold_uncertainty_score":0.008157432},"labels":[],"label_agreement":null},{"id":"W2772500632","doi":"10.3847/1538-4357/aaa1a0","title":"A Direct Measurement of Sense of Rotation of PSR J0737–3039A","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Angular momentum; Rotation (mathematics); Binary pulsar; Stellar rotation; Supernova; Millisecond pulsar; Orbit (dynamics)","score_opus":0.02085736052770542,"score_gpt":0.31539277500448754,"score_spread":0.2945354144767821,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2772500632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9648295,0.00015480752,0.026855042,0.000083549996,0.00006756394,0.00003675227,0.0009175039,0.0005167702,0.0065385583],"genre_scores_gemma":[0.97978055,0.000055609085,0.018731717,0.000019792586,0.000010662962,0.0000188993,0.0006534897,0.000059392347,0.00066987576],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998292,0.000025703972,0.000010498126,0.00006024024,0.000046487854,0.000027838829],"domain_scores_gemma":[0.9996648,0.000049011393,0.000070207854,0.00008694883,0.00007381574,0.000055307373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030412985,0.00022534974,0.00021217122,0.00085689535,0.00019132694,0.0005008056,0.00019013991,0.00024407708,0.0016954367],"category_scores_gemma":[0.001237381,0.00015253967,0.00020218283,0.0005958362,0.00024295032,0.00026641667,0.00042417922,0.0002964259,0.0010150688],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007216297,0.00008405009,0.32398644,0.00013267055,0.0001917883,0.00028594967,0.00044420236,0.008530893,0.47534072,0.0072675287,0.0032584583,0.17975557],"study_design_scores_gemma":[0.00007951819,0.00045214538,0.7383811,0.00003954025,0.000114819464,0.001304087,0.000398624,0.09665431,0.1420163,0.0035139818,0.016914,0.00013155532],"about_ca_topic_score_codex":0.0007368178,"about_ca_topic_score_gemma":0.0011008113,"teacher_disagreement_score":0.0016954367,"about_ca_system_score_codex":0.00017587532,"about_ca_system_score_gemma":0.0002522274,"threshold_uncertainty_score":0.0056717396},"labels":[],"label_agreement":null},{"id":"W2772671694","doi":"10.3847/1538-4357/aac770","title":"A Second Chromatic Timing Event of Interstellar Origin toward PSR J1713+0747","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; California Institute of Technology; National Aeronautics and Space Administration; Chinese Academy of Sciences; Universities Space Research Association; National Science Foundation","keywords":"Physics; Astrophysics; Line-of-sight; Interstellar medium; Pulsar; Pulse (music); Dispersion (optics); Residual; Event (particle physics); Optics; Galaxy; Detector; Mathematics","score_opus":0.024558225100029165,"score_gpt":0.34272322879654304,"score_spread":0.3181650036965139,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2772671694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99375796,0.00008710268,0.0010130159,0.00015784371,0.00007435175,0.000018040222,0.0004858939,0.00009328174,0.0043124813],"genre_scores_gemma":[0.9976871,0.000029571553,0.000579024,0.00006420685,0.000049775448,0.0000084337935,0.0006096263,0.000015492664,0.00095674547],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991286,0.0000054815855,0.0000046475225,0.000025894868,0.00002749272,0.000023612718],"domain_scores_gemma":[0.9994497,0.00008675422,0.0001335721,0.00008875742,0.00010529184,0.00013596064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016042293,0.00021089271,0.0001864354,0.0009883755,0.00070043537,0.00042619102,0.00026230584,0.00042347403,0.0023996718],"category_scores_gemma":[0.00048107642,0.00008238662,0.0002172037,0.00058730366,0.0002665668,0.00020219246,0.0005405606,0.00061932905,0.00034210275],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012153633,0.00035105695,0.5335578,0.00016410973,0.00021444583,0.014754152,0.0016501456,0.002097312,0.3841931,0.0082252305,0.0040541394,0.049523193],"study_design_scores_gemma":[0.000038010076,0.00033170008,0.9576735,0.000022705359,0.00006725811,0.0024651797,0.00027784018,0.0026432134,0.026696606,0.0006938699,0.009057968,0.000032168595],"about_ca_topic_score_codex":0.0055793985,"about_ca_topic_score_gemma":0.00799036,"teacher_disagreement_score":0.0055793985,"about_ca_system_score_codex":0.00066179014,"about_ca_system_score_gemma":0.00025203865,"threshold_uncertainty_score":0.011093855},"labels":[],"label_agreement":null},{"id":"W2773228766","doi":"10.3847/1538-4357/aa9aee","title":"Erratum: “First Search for Gravitational Waves from Known Pulsars with Advanced LIGO” (2017, ApJ, 839, 12)","year":2017,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; University of Pennsylvania","keywords":"LIGO; Physics; Gravitational wave; Pulsar; Astronomy; Gravitational-wave astronomy; Astrophysics; Gravitational-wave observatory","score_opus":0.019574244009600793,"score_gpt":0.3221548010522543,"score_spread":0.3025805570426535,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2773228766","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":"reproducibility","model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":"reproducibility","domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00033061736,0.00069485477,0.00018332282,0.05089917,0.9395596,0.000022546908,0.0013838903,0.00028855997,0.006637553],"genre_scores_gemma":[0.010642145,0.007531838,0.002287302,0.14909737,0.43739045,0.000181055,0.007829109,0.0019596186,0.38308108],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99754876,0.00021026023,0.0005448698,0.00031671565,0.001144287,0.00023509613],"domain_scores_gemma":[0.9896039,0.0024737641,0.0008701875,0.000809624,0.0054448587,0.00079771836],"candidate_categories":["metaresearch"],"consensus_categories":[],"category_scores_codex":[0.0021615278,0.0024485947,0.0015374317,0.0047041443,0.0055451086,0.004746923,0.002670493,0.00681194,0.050905377],"category_scores_gemma":[0.027959142,0.0009358583,0.0015492279,0.0022316321,0.002424613,0.00376765,0.0032217966,0.0093612345,0.050690796],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024618545,0.000008754403,0.00008000956,0.000043288226,0.0000047067524,0.00015088066,0.000014397854,0.000014651459,0.00005093988,0.00040558318,0.9970732,0.0021291135],"study_design_scores_gemma":[0.000036553254,0.000037036436,0.001669387,0.00027639445,0.000032186686,0.000407553,0.0001720336,0.00014091506,0.00044396514,0.0019406455,0.9947982,0.000045110988],"about_ca_topic_score_codex":0.01360211,"about_ca_topic_score_gemma":0.017016523,"teacher_disagreement_score":0.9978385,"about_ca_system_score_codex":0.003686441,"about_ca_system_score_gemma":0.0062065986,"threshold_uncertainty_score":0.17029548},"labels":[],"label_agreement":null},{"id":"W2773418845","doi":"10.3847/1538-4357/aaaf6b","title":"Future Cosmological Constraints From Fast Radio Bursts","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Redshift; Dark energy; Baryon; Equation of state; Intensity mapping; Curvature; COSMIC cancer database; Constraint (computer-aided design); Oscillation (cell signaling)","score_opus":0.012294047194614572,"score_gpt":0.30235431827993003,"score_spread":0.29006027108531546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2773418845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9650707,0.0009670961,0.02339923,0.00083057926,0.00003498942,0.000012135643,0.001175024,0.00012959781,0.008380605],"genre_scores_gemma":[0.9972145,0.00022897583,0.0017284884,0.000057810736,0.00003284693,0.0000030972717,0.00054082327,0.000013615849,0.00017990012],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99936706,0.00022207813,0.000027684167,0.0001533464,0.0001550546,0.00007472766],"domain_scores_gemma":[0.9896371,0.006302552,0.0020629081,0.00083489827,0.000608005,0.000554579],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021687474,0.000503915,0.00048562407,0.001051439,0.00046327547,0.0023194342,0.00051289523,0.00064736063,0.0027629752],"category_scores_gemma":[0.013880295,0.0004248291,0.00046102275,0.0010473751,0.00071151607,0.0017417363,0.00091446075,0.0007900614,0.00026908968],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038540465,0.00006574497,0.68747085,0.00020482241,0.0003093472,0.00041747084,0.00043544936,0.19974189,0.0073947925,0.0643788,0.0019383255,0.03725708],"study_design_scores_gemma":[0.00005313909,0.00012947679,0.46063292,0.00025620442,0.00016815995,0.00033504897,0.0004507403,0.4343369,0.0023415342,0.093740754,0.0074124993,0.00014273748],"about_ca_topic_score_codex":0.010153783,"about_ca_topic_score_gemma":0.00852008,"teacher_disagreement_score":0.010153783,"about_ca_system_score_codex":0.00081562554,"about_ca_system_score_gemma":0.00054668484,"threshold_uncertainty_score":0.020189345},"labels":[],"label_agreement":null},{"id":"W2773749868","doi":"10.3847/1538-4357/aa9e89","title":"A Radio Continuum and Polarization Study of SNR G57.2+0.8 Associated with Magnetar SGR 1935+2154","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Dominion Astrophysical Observatory; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Magnetar; Pulsar; Supernova remnant; Spectral index; Pulsar wind nebula; Milky Way; Polarization (electrochemistry); Magnetic field; Linear polarization","score_opus":0.005496456832607364,"score_gpt":0.19881958469310798,"score_spread":0.19332312786050063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2773749868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943465,0.000039748385,0.000072822055,0.000005349916,0.000001380214,0.000002148312,0.0000459751,0.00000557695,0.00039237022],"genre_scores_gemma":[0.99935883,0.000024582625,0.0001479666,0.000012543357,0.0000053658196,0.0000024550516,0.00021019607,0.0000028701857,0.00023534332],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995196,0.0000064847036,0.0000038635653,0.000012984833,0.00000869824,0.000016022987],"domain_scores_gemma":[0.9998584,0.000021803917,0.00003864735,0.000013277238,0.000023784027,0.00004406823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001430075,0.00023389219,0.00017774379,0.00093497144,0.00034784933,0.00031386354,0.00023540725,0.00017970763,0.0012662925],"category_scores_gemma":[0.00022495429,0.000088594665,0.00018286129,0.0003536555,0.00023166677,0.00011111904,0.00035309017,0.00012543639,0.00038773718],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011531801,0.0002578739,0.66094476,0.000052031734,0.000085427586,0.008008696,0.00045455876,0.00043578894,0.31759924,0.00020089668,0.00021959559,0.010588001],"study_design_scores_gemma":[0.000023384722,0.00054962886,0.9830383,0.000005209986,0.000039935814,0.0042942255,0.00029816004,0.00046682643,0.010383334,0.00006948125,0.00082338054,0.000008169183],"about_ca_topic_score_codex":0.0011779346,"about_ca_topic_score_gemma":0.0009831791,"teacher_disagreement_score":0.0012662925,"about_ca_system_score_codex":0.00017837145,"about_ca_system_score_gemma":0.00004917104,"threshold_uncertainty_score":0.0042362213},"labels":[],"label_agreement":null},{"id":"W2773917537","doi":"10.3847/1538-4357/aaa080","title":"Intensity-corrected Herschel Observations of Nearby Isolated Low-mass Clouds*","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; National Research Council Canada","funders":"","keywords":"Black-body radiation; Photometry (optics); Spectrometer; Intensity (physics); Offset (computer science); Measure (data warehouse); Molecular cloud","score_opus":0.016553734550221178,"score_gpt":0.24027907906268406,"score_spread":0.22372534451246287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2773917537","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994152,0.000109889355,0.0007719809,0.000044544828,0.0000056348913,0.000005919513,0.0019206001,0.00020959185,0.002779754],"genre_scores_gemma":[0.99522674,0.00004272569,0.0014264402,0.000025672492,0.00001224721,0.000007856805,0.0026491294,0.000058710248,0.00055046845],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981695,0.000013329287,0.0000066133935,0.00005447077,0.000057464495,0.00005126003],"domain_scores_gemma":[0.9996062,0.000039358427,0.0001003324,0.00009182239,0.00010885528,0.000053391792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026792157,0.00029183936,0.00028388176,0.0011467563,0.00044088485,0.00039797174,0.00041168166,0.00022266206,0.001994706],"category_scores_gemma":[0.00054272916,0.00016724481,0.00027105666,0.0010393377,0.000267298,0.00041073305,0.0006584797,0.00026516456,0.0006165128],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040740642,0.00013048672,0.8094175,0.00015918026,0.00027116624,0.0003468206,0.00076730584,0.022616586,0.105055705,0.0010249431,0.0054217475,0.054381214],"study_design_scores_gemma":[0.000033442822,0.000022373917,0.9755069,0.000011685818,0.00004292162,0.00006610902,0.00009611562,0.007987308,0.012033081,0.00016686399,0.0040094033,0.000023678287],"about_ca_topic_score_codex":0.012807811,"about_ca_topic_score_gemma":0.029916557,"teacher_disagreement_score":0.012807811,"about_ca_system_score_codex":0.00088346,"about_ca_system_score_gemma":0.0002476016,"threshold_uncertainty_score":0.025466561},"labels":[],"label_agreement":null},{"id":"W2778120926","doi":"10.3847/1538-4357/aad6ec","title":"r-process Nucleosynthesis from Three-dimensional Magnetorotational Core-collapse Supernovae","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":170,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Nucleosynthesis; Magnetohydrodynamic drive; Supernova; Magnetic field; Neutrino; Magnetorotational instability; Type II supernova; Magnetohydrodynamics; Neutron star","score_opus":0.015262713174387394,"score_gpt":0.24195387733503307,"score_spread":0.22669116416064566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2778120926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995265,0.000060892136,0.0016618988,0.00009549558,0.000011408846,0.000017758213,0.00021275204,0.00007839223,0.0025963036],"genre_scores_gemma":[0.99861515,0.000034640005,0.0008442335,0.00002860182,0.0000059344065,0.000015968044,0.00018687139,0.000025568599,0.00024298174],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998765,0.000036418984,0.000005674888,0.000015422886,0.000021791548,0.00004408126],"domain_scores_gemma":[0.9993864,0.0002017934,0.00011792235,0.000052985055,0.000074477175,0.00016637077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047908892,0.0006740993,0.00061957876,0.00040074342,0.0006786214,0.0008353995,0.0010003443,0.00070130173,0.0012180819],"category_scores_gemma":[0.0016253686,0.00040237207,0.0008828351,0.00042970566,0.0009238916,0.0004089918,0.0008587112,0.00063792954,0.00012569634],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018334342,0.00006938375,0.007360429,0.00002125595,0.00006775393,0.00016061177,0.00004868218,0.98624843,0.0033088087,0.001850221,0.00013011774,0.00055099075],"study_design_scores_gemma":[0.00008738892,0.0000612698,0.003830683,0.00000391557,0.000017137756,0.000020812864,0.000028239085,0.99373734,0.0011132114,0.00097297045,0.00011266296,0.000014313164],"about_ca_topic_score_codex":0.024258064,"about_ca_topic_score_gemma":0.011087291,"teacher_disagreement_score":0.024258064,"about_ca_system_score_codex":0.0013370349,"about_ca_system_score_gemma":0.0010112455,"threshold_uncertainty_score":0.048233747},"labels":[],"label_agreement":null},{"id":"W2779221820","doi":"10.3847/1538-4357/aaaae8","title":"i-process Contribution of Rapidly Accreting White Dwarfs to the Solar Composition of First-peak Neutron-capture Elements","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Metallicity; Galaxy; s-process; White dwarf; Nucleosynthesis; Solar mass; Isotope; Stellar evolution; Astronomy; Stellar mass; Population; Stars; Star formation; Nuclear physics","score_opus":0.007327749661037137,"score_gpt":0.23999649516974042,"score_spread":0.23266874550870328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2779221820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9885916,0.0002711784,0.008408162,0.000045164343,0.000017989976,0.000008545137,0.0003223577,0.00023312941,0.0021018398],"genre_scores_gemma":[0.9980896,0.0000776603,0.0010068634,0.00001943332,0.0000056596864,0.000004250159,0.0004100941,0.00006671162,0.00031968692],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996717,0.000049829156,0.00001817463,0.00011675557,0.000098321616,0.000045227185],"domain_scores_gemma":[0.9992067,0.0002565021,0.00017646339,0.00016846975,0.00012080671,0.00007114632],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00080192846,0.00070868875,0.0004079922,0.00084343116,0.00028718874,0.00090720045,0.0007200701,0.00047037538,0.0010824606],"category_scores_gemma":[0.0017835457,0.00032202885,0.0009376929,0.00039154635,0.00034516945,0.00045776932,0.00072567724,0.0003007167,0.00033733415],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084251375,0.00008345588,0.70571214,0.000252433,0.00048658965,0.0007344408,0.00021501038,0.085365154,0.17494376,0.0063894643,0.0004554056,0.02451967],"study_design_scores_gemma":[0.00013318002,0.0004314938,0.48737982,0.00005824433,0.00047286128,0.001089423,0.00023642535,0.30750737,0.19009703,0.0068727992,0.005632344,0.0000890459],"about_ca_topic_score_codex":0.0025903706,"about_ca_topic_score_gemma":0.0014064299,"teacher_disagreement_score":0.0025903706,"about_ca_system_score_codex":0.0007015273,"about_ca_system_score_gemma":0.00023383464,"threshold_uncertainty_score":0.0051505566},"labels":[],"label_agreement":null},{"id":"W2779391643","doi":"10.3847/1538-4357/aaa290","title":"A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces. I. Cloud-scale Gas Motions","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Star formation; Galaxy; Molecular cloud; Spiral galaxy; Galactic plane; Virial theorem; Gravitational potential; Gravitational collapse; Stars","score_opus":0.0094337218169669,"score_gpt":0.2399829913364825,"score_spread":0.2305492695195156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2779391643","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.52388877,0.0036747348,0.3291397,0.0114599755,0.00053566264,0.0003649968,0.0012743905,0.0008019029,0.12885988],"genre_scores_gemma":[0.95873016,0.0009994407,0.013089616,0.00059159816,0.00017669261,0.0002683537,0.00015508596,0.000096126045,0.025892977],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989784,0.000023426108,0.000005028882,0.000029402401,0.000017107797,0.000027173957],"domain_scores_gemma":[0.9997893,0.00004356772,0.00005234258,0.000017725182,0.000024856261,0.00007219584],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026020975,0.0005608254,0.00050231494,0.0005501846,0.00069489266,0.0013023751,0.0019575227,0.0023301877,0.0056367693],"category_scores_gemma":[0.00053680775,0.00036926437,0.0009564374,0.0003087852,0.0013838157,0.0018570706,0.0011967476,0.0008127464,0.0012296418],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000078550496,0.00009670616,0.006345088,0.0001307949,0.00005101483,0.0007464525,0.00041755493,0.3660618,0.013974396,0.60215974,0.0032348363,0.0067030173],"study_design_scores_gemma":[0.00007802158,0.000093231625,0.0027250496,0.000024029208,0.000020444733,0.0002506063,0.00009751879,0.8595563,0.000405821,0.1317568,0.00495885,0.000033394674],"about_ca_topic_score_codex":0.0053870706,"about_ca_topic_score_gemma":0.002838663,"teacher_disagreement_score":0.0056367693,"about_ca_system_score_codex":0.0013117115,"about_ca_system_score_gemma":0.0006337056,"threshold_uncertainty_score":0.018856883},"labels":[],"label_agreement":null},{"id":"W2779538294","doi":"10.3847/1538-4357/aab4f8","title":"A Search for Neutrino Emission from Fast Radio Bursts with Six Years of IceCube Data","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Snolab; University of Alberta","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Physics; Neutrino; Astrophysics; Coincidence; Sky; Astronomy; Neutrino detector; Neutrino oscillation; Nuclear physics","score_opus":0.020171210241454324,"score_gpt":0.2622033156859826,"score_spread":0.24203210544452827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2779538294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994263,0.00026282817,0.0027045275,0.000047896985,0.000010919314,0.000016770795,0.0015851278,0.00007743046,0.001031511],"genre_scores_gemma":[0.99039054,0.000103330596,0.0032005196,0.000024831668,0.00002169466,0.000022939228,0.005990845,0.000037727023,0.00020753662],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99888486,0.00029120158,0.000087829874,0.00030601336,0.00023842641,0.00019161684],"domain_scores_gemma":[0.9953506,0.001964278,0.0014709125,0.00045015416,0.00034562493,0.00041835938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032308546,0.00041976254,0.0005663391,0.0019454058,0.00058155815,0.0013645601,0.0005259572,0.00055519195,0.0012079139],"category_scores_gemma":[0.0044452893,0.00029607225,0.000635125,0.002082296,0.00030626325,0.00046666677,0.0008691401,0.00036702683,0.0002279807],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011429747,0.00012391762,0.9596164,0.00008622485,0.00050811307,0.0009944102,0.00022386087,0.006168375,0.016228031,0.0005351983,0.0008440979,0.013528262],"study_design_scores_gemma":[0.00006285412,0.00038006515,0.9579533,0.000036655594,0.00027373421,0.0013831989,0.00023888414,0.021844823,0.01205358,0.00057141605,0.005162154,0.00003940808],"about_ca_topic_score_codex":0.0036193857,"about_ca_topic_score_gemma":0.0044271126,"teacher_disagreement_score":0.0036193857,"about_ca_system_score_codex":0.0005186618,"about_ca_system_score_gemma":0.00065947854,"threshold_uncertainty_score":0.017086625},"labels":[],"label_agreement":null},{"id":"W2780207415","doi":"10.3847/1538-4357/aac264","title":"Constraints on Cosmological Parameters from the Angular Power Spectrum of a Combined 2500 deg<sup>2</sup> SPT-SZ and Planck Gravitational Lensing Map","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Physics; Cosmic microwave background; Planck; Astrophysics; South Pole Telescope; Spectral density; Gravitational lens; Omega; Weak gravitational lensing; Lambda; Dark energy; Cold dark matter; Dark matter; Cosmology; Redshift; Galaxy; Quantum mechanics; Statistics; Anisotropy","score_opus":0.010633030030829518,"score_gpt":0.23469432801437354,"score_spread":0.22406129798354402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2780207415","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9899979,0.00008057403,0.006156458,0.0000668179,0.0000050732497,0.000004108591,0.0015979665,0.00010468842,0.0019863797],"genre_scores_gemma":[0.9961738,0.000038341357,0.0017185723,0.00001320881,0.000009828777,0.0000048039196,0.001884698,0.000041319454,0.00011548379],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994654,0.00013539345,0.00002489451,0.00010542905,0.00021058468,0.000058409143],"domain_scores_gemma":[0.9963085,0.0017033126,0.00065597164,0.000671706,0.00037291663,0.0002874938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013027157,0.00090718735,0.0005914684,0.0012218539,0.00031714758,0.0011530663,0.0005916097,0.0003588837,0.0032352803],"category_scores_gemma":[0.0054839617,0.00049172324,0.0009770814,0.001704475,0.00049936556,0.0007624014,0.0007792209,0.0003808193,0.00078842515],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013761827,0.00008562573,0.7058175,0.00022805236,0.0014268071,0.0010891064,0.00037325954,0.15656202,0.09077604,0.0066730524,0.0025655087,0.033026844],"study_design_scores_gemma":[0.000051642575,0.000073993135,0.8519102,0.0000311854,0.00032108492,0.00040900105,0.00014209044,0.12480893,0.015596248,0.0031516857,0.0034231066,0.0000807763],"about_ca_topic_score_codex":0.0052715433,"about_ca_topic_score_gemma":0.0049991333,"teacher_disagreement_score":0.0052715433,"about_ca_system_score_codex":0.00046576682,"about_ca_system_score_gemma":0.00025528713,"threshold_uncertainty_score":0.010823071},"labels":[],"label_agreement":null},{"id":"W2781656774","doi":"10.3847/1538-4357/aad283","title":"A Projected Estimate of the Reionization Optical Depth Using the CLASS Experiment’s Sample Variance Limited E-mode Measurement","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Division of Astronomical Sciences; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Maryland Advanced Research Computing Center; National Science Foundation","keywords":"Cosmic microwave background; Reionization; Cosmic variance; Cosmology; Cosmic background radiation; Sample variance; Multipole expansion; COSMIC cancer database; Gravitational lens; Optical depth","score_opus":0.03258305908204007,"score_gpt":0.30710249605242085,"score_spread":0.2745194369703808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2781656774","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9555906,0.000077008175,0.038540844,0.0001414549,0.000012434595,0.000018237553,0.0012815665,0.00041333918,0.0039246385],"genre_scores_gemma":[0.99201125,0.00001413038,0.007245495,0.000016887643,0.000005149939,0.000008791711,0.00048089316,0.000031656393,0.00018569067],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997093,0.000108740125,0.0000071952077,0.00007171796,0.00006356101,0.000039528462],"domain_scores_gemma":[0.9976554,0.0010723666,0.00035946135,0.0004765701,0.00028478232,0.00015136276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015047523,0.0002045855,0.00020105092,0.00051841885,0.00022070609,0.00049779133,0.00040604267,0.00026308853,0.0014979765],"category_scores_gemma":[0.0050218552,0.00021103452,0.00034270764,0.00036330786,0.00026900324,0.00046507007,0.00051589473,0.00031368012,0.00019756083],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018388014,0.00017667373,0.5755154,0.00009818681,0.00047951992,0.00021521223,0.00019649528,0.29976058,0.040862516,0.017764647,0.0031137024,0.059978195],"study_design_scores_gemma":[0.00011614802,0.00013418638,0.28934336,0.000022092358,0.000074799376,0.0001887978,0.00005923871,0.68138236,0.016053332,0.008950807,0.0035986179,0.000076262004],"about_ca_topic_score_codex":0.004605832,"about_ca_topic_score_gemma":0.0054750955,"teacher_disagreement_score":0.004605832,"about_ca_system_score_codex":0.0004884802,"about_ca_system_score_gemma":0.00029817218,"threshold_uncertainty_score":0.009158015},"labels":[],"label_agreement":null},{"id":"W2781930916","doi":"10.3847/1538-4357/aaa3e6","title":"Revisiting the Extended Schmidt Law: The Important Role of Existing Stars in Regulating Star Formation","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Star formation; Spiral galaxy; Stars; Galaxy; Dwarf galaxy; Star cluster; Irregular galaxy; Stellar mass; Molecular cloud","score_opus":0.01790220341332982,"score_gpt":0.26864681710923993,"score_spread":0.2507446136959101,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2781930916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95864505,0.0011355412,0.032573503,0.00046461402,0.000031073705,0.000017847226,0.00009839162,0.00021400838,0.0068199136],"genre_scores_gemma":[0.99786407,0.00015355008,0.0015131879,0.000046338817,0.000023017832,0.0000037842558,0.0000304574,0.00001056262,0.00035498574],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996425,0.00005723669,0.000020114745,0.00011140782,0.00012120753,0.00004752824],"domain_scores_gemma":[0.99788576,0.00061090954,0.00049559854,0.00041522534,0.00035772446,0.00023478876],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009816866,0.00025974849,0.00038859455,0.00062131166,0.0002663534,0.00075671944,0.0007552156,0.0003532385,0.001503759],"category_scores_gemma":[0.0041692345,0.00014948164,0.00024145255,0.00035460078,0.0014930967,0.0014779951,0.00089245656,0.00047953372,0.0003380616],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005661064,0.00020467937,0.5081134,0.00031228273,0.00019052876,0.001119772,0.0012341114,0.06088834,0.10656634,0.16781539,0.003734496,0.14925458],"study_design_scores_gemma":[0.000063351814,0.000610855,0.5116886,0.00006711089,0.00006847658,0.0014654048,0.00063803,0.29097533,0.019030118,0.16806902,0.007210121,0.00011356593],"about_ca_topic_score_codex":0.0016223398,"about_ca_topic_score_gemma":0.0010573117,"teacher_disagreement_score":0.0016223398,"about_ca_system_score_codex":0.00032060163,"about_ca_system_score_gemma":0.0003446348,"threshold_uncertainty_score":0.0051917434},"labels":[],"label_agreement":null},{"id":"W2781996299","doi":"10.3847/1538-4357/aa9c82","title":"The Solar-flux Third Granulation Signature","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Spectrograph; Flux (metallurgy); Spectral resolution; Line (geometry); Wavelength; Spectral line; Astronomy; Optics; Geometry","score_opus":0.005077412078436363,"score_gpt":0.22325846085480672,"score_spread":0.21818104877637035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2781996299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9896465,0.000071597664,0.004408654,0.000021968799,0.000009384623,0.000008950378,0.00065370154,0.00023707416,0.0049422304],"genre_scores_gemma":[0.9977616,0.000018528119,0.0012319346,0.000012058248,0.000003075878,0.000004387304,0.00048457735,0.000027201579,0.00045665816],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997553,0.000024422161,0.000016497494,0.000044363187,0.00012834992,0.000031084834],"domain_scores_gemma":[0.9979085,0.00040393707,0.00053711707,0.00034131992,0.0006377623,0.00017142229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032605787,0.000103444436,0.00018993698,0.0012146322,0.00022638794,0.0007885548,0.0001883063,0.00018974909,0.0015865709],"category_scores_gemma":[0.0016887473,0.000090224275,0.00018209885,0.0007113659,0.0002578864,0.00036460676,0.00048945873,0.00021550967,0.00045716338],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083647226,0.00006889215,0.77269256,0.00009864185,0.000083498024,0.00023878516,0.0006333727,0.0032059862,0.11190376,0.0017495179,0.0014229341,0.107065514],"study_design_scores_gemma":[0.000009269138,0.00011581932,0.9513711,0.000010435714,0.000027264667,0.0004441142,0.00013005063,0.0062527107,0.037093256,0.000825237,0.0036994717,0.0000211853],"about_ca_topic_score_codex":0.001319384,"about_ca_topic_score_gemma":0.0011477558,"teacher_disagreement_score":0.0015865709,"about_ca_system_score_codex":0.0003457178,"about_ca_system_score_gemma":0.000098700584,"threshold_uncertainty_score":0.005307555},"labels":[],"label_agreement":null},{"id":"W2782085449","doi":"10.3847/1538-4357/aad18b","title":"Effect of Template Uncertainties on the WMAP and Planck Measures of the Optical Depth Due to Reionization","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Reionization; CMB cold spot; Cosmic microwave background; Planck; Cosmic background radiation; Polarization (electrochemistry); Cosmic variance; Anisotropy","score_opus":0.010311152560502867,"score_gpt":0.2514635016388013,"score_spread":0.24115234907829847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2782085449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.972388,0.00071849185,0.017956229,0.00031647322,0.00007439433,0.000030152314,0.0037336685,0.0002573741,0.004525091],"genre_scores_gemma":[0.99673426,0.000056348086,0.001582403,0.000063233485,0.00001558347,0.000014999947,0.0012692129,0.000074457115,0.00018960272],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99504375,0.0021695956,0.00040181566,0.0013598512,0.0007366304,0.00028840796],"domain_scores_gemma":[0.9244241,0.053473655,0.0075048925,0.010859289,0.0028477262,0.0008902867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010254616,0.0005320175,0.00031563244,0.000983903,0.0004313265,0.0014955819,0.0008009727,0.0005035796,0.001495777],"category_scores_gemma":[0.051423702,0.0004056811,0.0010398345,0.001745836,0.00071855646,0.0010932091,0.0010587611,0.00059915,0.00030945538],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053404504,0.000051469546,0.923911,0.00011910999,0.001812868,0.00021894582,0.00049887423,0.041536536,0.004025938,0.0039197817,0.0020496245,0.021321887],"study_design_scores_gemma":[0.000028243643,0.00012745561,0.94691527,0.00011247833,0.00048445564,0.0002144989,0.00039144506,0.03177374,0.012119282,0.0032727618,0.0044698482,0.00009052475],"about_ca_topic_score_codex":0.011236335,"about_ca_topic_score_gemma":0.006581873,"teacher_disagreement_score":0.011236335,"about_ca_system_score_codex":0.00067956984,"about_ca_system_score_gemma":0.0005013936,"threshold_uncertainty_score":0.0542323},"labels":[],"label_agreement":null},{"id":"W2782663518","doi":"10.3847/1538-4357/aa911f","title":"The JCMT Gould Belt Survey: A First Look at the Auriga–California Molecular Cloud with SCUBA-2","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Manitoba; University of Waterloo; Herzberg Institute of Astrophysics; University of Alberta; Université Laval; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Protostar; Physics; Astrophysics; Star formation; Molecular cloud; Young stellar object; Astronomy; James Clerk Maxwell Telescope; Stars","score_opus":0.008283605569583668,"score_gpt":0.22542678475557038,"score_spread":0.21714317918598672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2782663518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98575145,0.00024418294,0.00016006184,0.000091949965,0.0000066799685,0.000045492627,0.009043796,0.000089161,0.004567129],"genre_scores_gemma":[0.9848663,0.0002190995,0.0013867026,0.00010127025,0.000024734787,0.000035419256,0.012103276,0.000033050288,0.0012300928],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998078,0.000010760892,0.000009880242,0.000053313506,0.000077527206,0.000040856386],"domain_scores_gemma":[0.99931264,0.00003688479,0.00018651035,0.00010018659,0.00016901338,0.00019464364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017772276,0.00015905985,0.00017019163,0.0023510007,0.00053592,0.0005767329,0.00043954072,0.00015905288,0.0016642801],"category_scores_gemma":[0.0005503823,0.0001219546,0.00012430476,0.0017155821,0.0001633111,0.00027318383,0.00063146517,0.00018265356,0.0003191342],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000038514885,0.00003077218,0.98590696,0.000025993062,0.000030846102,0.00012894912,0.00026622173,0.000080498445,0.0042903326,0.0000595473,0.0028034183,0.0063379006],"study_design_scores_gemma":[0.0000025142988,0.000004382385,0.9978441,0.0000058618807,0.000006362507,0.000034280576,0.00008693967,0.000098663535,0.0001701511,0.000004891054,0.00174004,0.000001810099],"about_ca_topic_score_codex":0.13873878,"about_ca_topic_score_gemma":0.34080017,"teacher_disagreement_score":0.13873878,"about_ca_system_score_codex":0.00065742026,"about_ca_system_score_gemma":0.00048217774,"threshold_uncertainty_score":0.27586246},"labels":[],"label_agreement":null},{"id":"W2782863415","doi":"10.3847/1538-4357/aa9feb","title":"Wide-field Imaging of the Environments of LITTLE THINGS Dwarf Irregular Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Dwarf galaxy; Astrophysics; Astronomy; Galaxy; Luminous infrared galaxy; Irregular galaxy; Star formation; Luminosity; Local Group; Interacting galaxy","score_opus":0.004484056422850446,"score_gpt":0.1945549317577617,"score_spread":0.19007087533491127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2782863415","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971861,0.00007565073,0.0006244796,0.000015682648,0.000001967297,0.0000038902363,0.00022117609,0.000036924746,0.0018339561],"genre_scores_gemma":[0.9982937,0.000029627086,0.0010621303,0.000016110425,0.000005211747,0.0000023204534,0.00032430823,0.000010183234,0.00025641292],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998987,0.00001028785,0.0000038429102,0.000032531803,0.000025902455,0.000028795757],"domain_scores_gemma":[0.9994242,0.00009347827,0.00011393726,0.000107505344,0.00008362119,0.000177339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002441348,0.000103225284,0.00015461896,0.0010859154,0.00032355954,0.00032804714,0.00017782854,0.00018162008,0.0012264252],"category_scores_gemma":[0.00043833378,0.00016292474,0.00012934745,0.00046075392,0.00025440683,0.0002628629,0.00047585048,0.00015494217,0.00024328112],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005981504,0.000080173486,0.603113,0.000079420184,0.00012721676,0.0008978205,0.0012274642,0.00095718075,0.35903427,0.0005530958,0.0010832953,0.03224898],"study_design_scores_gemma":[0.000007211383,0.00005433793,0.9916596,0.000005674738,0.000016466172,0.0004139262,0.00023624714,0.000487564,0.0055867466,0.00013624203,0.0013881045,0.000008097104],"about_ca_topic_score_codex":0.002341258,"about_ca_topic_score_gemma":0.0062701544,"teacher_disagreement_score":0.002341258,"about_ca_system_score_codex":0.00016496883,"about_ca_system_score_gemma":0.000066895474,"threshold_uncertainty_score":0.0046553016},"labels":[],"label_agreement":null},{"id":"W2782872280","doi":"10.3847/1538-4357/aaa5a4","title":"Quenching or Bursting: The Role of Stellar Mass, Environment, and Specific Star Formation Rate to","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; York University; Office of Science; Johns Hopkins University; Science and Technology Facilities Council; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; Vanderbilt University; University of Portsmouth; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy; National Science Foundation","keywords":"Bursting; Physics; Quenching (fluorescence); Galaxy; Astrophysics; Sigma; Star formation; Star (game theory); Stellar mass; Astronomy; Quantum mechanics","score_opus":0.008935287560797799,"score_gpt":0.19873545165862672,"score_spread":0.1898001640978289,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2782872280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937963,0.0000600653,0.00030160634,0.000011977825,5.377224e-7,0.00000195325,0.00007992382,0.000008603994,0.00015574985],"genre_scores_gemma":[0.9996582,0.000013265874,0.00012896354,0.000008562781,0.0000017348497,0.0000012694331,0.00011727894,0.0000026500945,0.00006809447],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986553,0.00003862817,0.000006693801,0.000046529727,0.000016150787,0.0000263784],"domain_scores_gemma":[0.9977506,0.00065618387,0.0008427882,0.00026431063,0.00012691949,0.00035915436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067553023,0.00019723862,0.00027686125,0.0006168084,0.00017345414,0.0005048922,0.00030419335,0.00020891098,0.0008554033],"category_scores_gemma":[0.0020408838,0.00009426618,0.00024525487,0.00040126292,0.00032255088,0.000327148,0.0003880197,0.0002556525,0.00013982833],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011546096,0.000021600621,0.98824966,0.000007876723,0.00006830184,0.000028469809,0.00011120867,0.0007876281,0.0061718696,0.00013063182,0.000041802316,0.0042654774],"study_design_scores_gemma":[0.0000020910538,0.000038787253,0.99623674,0.0000011461866,0.000012585007,0.000033004828,0.000032028354,0.002863201,0.0005831693,0.0000917861,0.00010285263,0.0000025542888],"about_ca_topic_score_codex":0.0025676358,"about_ca_topic_score_gemma":0.0022692268,"teacher_disagreement_score":0.0025676358,"about_ca_system_score_codex":0.00021094599,"about_ca_system_score_gemma":0.00006747433,"threshold_uncertainty_score":0.005105436},"labels":[],"label_agreement":null},{"id":"W2782895736","doi":"10.3847/1538-4357/aaa295","title":"OGLE-2014-BLG-0289: Precise Characterization of a Quintuple-peak Gravitational Microlensing Event","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Japan Society for the Promotion of Science; Narodowym Centrum Nauki; National Aeronautics and Space Administration; Korea Research Environment Open Network; National Research Foundation of Korea; Korea Institute of Science and Technology; Jet Propulsion Laboratory; National Research Foundation; Science and Technology Facilities Council; Korea Institute of Science and Technology Information; NASA Exoplanet Science Institute; California Institute of Technology","keywords":"Gravitational microlensing; Caustic (mathematics); Light curve; Parallax; Einstein radius; Event (particle physics); Measure (data warehouse); Occultation; Gravitational lens","score_opus":0.0060462611548660955,"score_gpt":0.24573748127838552,"score_spread":0.23969122012351943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2782895736","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9674769,0.00036826296,0.012375521,0.00024409126,0.00006125751,0.00008700571,0.0052819266,0.0015245598,0.0125803845],"genre_scores_gemma":[0.98661137,0.00004596673,0.005975742,0.000108253924,0.000034792272,0.000023603341,0.0062654507,0.00031336263,0.0006215193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996269,0.000028387383,0.000015840089,0.00012112891,0.00012628779,0.00008145918],"domain_scores_gemma":[0.9988951,0.0001673715,0.0003019691,0.00023595152,0.00014301934,0.00025663959],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00064845546,0.0004752856,0.0006056207,0.0017354848,0.0006950811,0.0016704688,0.00040937346,0.0005912872,0.0021577987],"category_scores_gemma":[0.001130178,0.00030164875,0.0005635249,0.0013316396,0.00030290178,0.0003366075,0.0011396229,0.00071583455,0.00079645816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026204498,0.00054344046,0.6585337,0.00041230832,0.00059053174,0.0077137067,0.0012349725,0.022087084,0.19640759,0.014883246,0.01512636,0.07984661],"study_design_scores_gemma":[0.000119420474,0.00019346164,0.9159729,0.000041866515,0.00010726621,0.0018057742,0.00020900743,0.04371284,0.020178776,0.0027994155,0.014760638,0.00009866016],"about_ca_topic_score_codex":0.0034014985,"about_ca_topic_score_gemma":0.005278151,"teacher_disagreement_score":0.0034014985,"about_ca_system_score_codex":0.00087563455,"about_ca_system_score_gemma":0.00036085327,"threshold_uncertainty_score":0.0072185993},"labels":[],"label_agreement":null},{"id":"W2783015515","doi":"10.3847/1538-4357/aaa764","title":"The JCMT Transient Survey: Stochastic and Secular Variability of Protostars and Disks In the Submillimeter Region Observed over 18 Months","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Brightness; Gaussian; Protostar; Distribution (mathematics); Luminosity; Apparent magnitude","score_opus":0.028031988247978347,"score_gpt":0.2543413950458418,"score_spread":0.22630940679786346,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783015515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990532,0.00003869896,0.000110231296,0.000010949594,0.0000012826587,0.000004360493,0.00063502614,0.000018320776,0.0001278792],"genre_scores_gemma":[0.99801946,0.000026662608,0.00018246198,0.000008464939,0.000009677226,0.000007461382,0.0016687334,0.000008694097,0.00006842873],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99961936,0.00004560656,0.000035227877,0.000090913556,0.00011763181,0.00009124693],"domain_scores_gemma":[0.9964139,0.00043634267,0.0017800056,0.00038672017,0.000406573,0.0005764194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006031564,0.00024725244,0.00037742755,0.0021851438,0.00045560766,0.00065760355,0.000357861,0.00036835094,0.0004965485],"category_scores_gemma":[0.0023599076,0.000181745,0.00039587394,0.0018737564,0.00031427492,0.00037215772,0.00068006094,0.00025500034,0.00018281056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006673698,0.000022486569,0.99521506,0.000007438671,0.00004984331,0.00010805366,0.000088501976,0.00027183266,0.0024269102,0.000018049572,0.00015909314,0.0015660146],"study_design_scores_gemma":[0.0000015150671,0.000015726295,0.99909675,0.00000118145,0.000007784433,0.0000697122,0.000021746477,0.0005050998,0.0001714893,0.0000034660527,0.000103754945,0.0000017487346],"about_ca_topic_score_codex":0.015045893,"about_ca_topic_score_gemma":0.020655308,"teacher_disagreement_score":0.015045893,"about_ca_system_score_codex":0.0005644487,"about_ca_system_score_gemma":0.00026180412,"threshold_uncertainty_score":0.029916584},"labels":[],"label_agreement":null},{"id":"W2783195820","doi":"10.3847/1538-4357/aabd3b","title":"The NANOGrav 11 Year Data Set: Pulsar-timing Constraints on the Stochastic Gravitational-wave Background","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":412,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"","keywords":"Gravitational wave background; Gravitational wave; Ephemeris; Pulsar; Population; Observatory; Amplitude; Eccentricity (behavior); Scaling","score_opus":0.07701501360039699,"score_gpt":0.3603458093083563,"score_spread":0.2833307957079593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783195820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9384068,0.00020535053,0.0022320936,0.00028677777,0.00005801836,0.000030828483,0.051828757,0.00015790136,0.00679345],"genre_scores_gemma":[0.85793674,0.0000862307,0.0035364213,0.00015687587,0.00004557679,0.00005682107,0.13635817,0.00008438594,0.0017386965],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992644,0.00009437828,0.0000610972,0.0001956121,0.00030851655,0.00007598334],"domain_scores_gemma":[0.9968491,0.0005412834,0.0008421387,0.000888181,0.0005199409,0.00035932005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012677442,0.00024388515,0.0003983372,0.0017233094,0.00040186028,0.00087321043,0.00058591814,0.00031763685,0.001738132],"category_scores_gemma":[0.0030494104,0.00018102827,0.00028001363,0.0020121587,0.00025720376,0.0005635902,0.0013381004,0.00044951594,0.0007469068],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041555692,0.000088912624,0.95809454,0.00007489401,0.00015597003,0.0002178753,0.0001693034,0.00547814,0.0057299924,0.0017998558,0.012200033,0.015574909],"study_design_scores_gemma":[0.000051988587,0.00005263433,0.95800203,0.000028934517,0.00004332122,0.00012928282,0.00012955412,0.008621795,0.002171068,0.00055647915,0.030180594,0.00003238726],"about_ca_topic_score_codex":0.014840855,"about_ca_topic_score_gemma":0.045153815,"teacher_disagreement_score":0.014840855,"about_ca_system_score_codex":0.000451027,"about_ca_system_score_gemma":0.00045917608,"threshold_uncertainty_score":0.029508889},"labels":[],"label_agreement":null},{"id":"W2783368210","doi":"10.3847/1538-4357/aaa95a","title":"A Radio Frequency Study of the Accreting Millisecond X-ray Pulsar, IGR J16597–3704, in the Globular Cluster NGC 6256","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Jansky; Millisecond pulsar; Neutron star; Astronomy; Radio telescope; Luminosity; Pulsar; Galaxy; Radio galaxy","score_opus":0.013020704689737251,"score_gpt":0.24352827150300138,"score_spread":0.23050756681326412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783368210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99973565,0.00002478269,0.000035248642,0.00000397771,8.0251283e-7,9.3392254e-7,0.000031917403,0.0000010867994,0.00016551024],"genre_scores_gemma":[0.9995466,0.00002584937,0.000088962646,0.000005296417,0.0000036109261,0.0000011706817,0.00012889504,8.709929e-7,0.00019871794],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999268,0.000008210958,0.0000054454335,0.000023018607,0.000018743807,0.000017756045],"domain_scores_gemma":[0.99979585,0.00002194321,0.00007469308,0.000018590166,0.000027310822,0.00006155194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018730601,0.00013765515,0.00012636115,0.00081061356,0.00035869508,0.00028482464,0.00018293227,0.00013440977,0.00077645987],"category_scores_gemma":[0.0003146098,0.00010313015,0.000108574444,0.00051045226,0.0002642789,0.00016254146,0.00036105202,0.00010780421,0.00022395104],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022648097,0.00005841294,0.9407179,0.000014633458,0.000039081253,0.0005428951,0.00048039143,0.00019723113,0.052284393,0.000105871666,0.000095579344,0.0052370713],"study_design_scores_gemma":[0.000004283115,0.00004241902,0.9988881,0.0000012405269,0.0000063795474,0.0001525998,0.0001270688,0.00010048327,0.00051455625,0.000015628155,0.00014585441,0.0000013870406],"about_ca_topic_score_codex":0.008317293,"about_ca_topic_score_gemma":0.011604383,"teacher_disagreement_score":0.008317293,"about_ca_system_score_codex":0.00022212454,"about_ca_system_score_gemma":0.00010149473,"threshold_uncertainty_score":0.016537786},"labels":[],"label_agreement":null},{"id":"W2783493734","doi":"10.3847/1538-4357/aaa4f7","title":"Role of Core-collapse Supernovae in Explaining Solar System Abundances of p Nuclides","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency; Compute Canada; Canarie; Canadian Foundation for AIDS Research; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; National Science Foundation","keywords":"Nucleosynthesis; Nuclide; Supernova; Metallicity; Big Bang nucleosynthesis; Solar System; Stellar nucleosynthesis; Nuclear reaction; r-process","score_opus":0.012559345259249483,"score_gpt":0.2352903102128716,"score_spread":0.22273096495362213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783493734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905515,0.0005860268,0.0058981306,0.00007669863,0.000017868435,0.000014794591,0.0003553402,0.00008817567,0.0024116223],"genre_scores_gemma":[0.9988906,0.00013369779,0.00051377295,0.000008427411,0.0000056721697,0.0000030608455,0.00016135076,0.000022906983,0.00026036287],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99988306,0.000030855605,0.000007594686,0.00003774898,0.000022109352,0.000018612936],"domain_scores_gemma":[0.99925333,0.0003748393,0.00011516469,0.00007805098,0.000076310585,0.00010222164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072604284,0.00051333057,0.00031554757,0.00071319664,0.00029896293,0.0008283941,0.0005743878,0.0004726787,0.0011179898],"category_scores_gemma":[0.002341089,0.00025445924,0.000586464,0.0003735,0.0003496557,0.00053724437,0.0005169501,0.0002857121,0.0002480789],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026766007,0.000081814775,0.70622724,0.00017153179,0.00046252186,0.0006350279,0.00012764141,0.24207188,0.028610623,0.006997896,0.00038126897,0.013964864],"study_design_scores_gemma":[0.000019580362,0.00009295697,0.25479198,0.000038904753,0.00012379124,0.00024993118,0.00010819363,0.73213357,0.0052047186,0.0052819815,0.0019322877,0.000022076669],"about_ca_topic_score_codex":0.0069688857,"about_ca_topic_score_gemma":0.0061576413,"teacher_disagreement_score":0.0069688857,"about_ca_system_score_codex":0.0004780001,"about_ca_system_score_gemma":0.00028013138,"threshold_uncertainty_score":0.013856649},"labels":[],"label_agreement":null},{"id":"W2783859845","doi":"10.3847/1538-4357/aacce8","title":"Cool-core Clusters: The Role of BCG, Star Formation, and AGN-driven Turbulence","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Intracluster medium; Turbulence; Jet (fluid); Cluster (spacecraft); Star formation; Active galactic nucleus; Core (optical fiber); Star cluster","score_opus":0.011536092834546373,"score_gpt":0.25695866112486576,"score_spread":0.2454225682903194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783859845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99831676,0.000115446375,0.00045651355,0.00009912507,0.000013641198,0.0000065355257,0.00013169613,0.00006321073,0.0007970162],"genre_scores_gemma":[0.99930406,0.000031811112,0.00035281258,0.000019885463,0.0000072268617,0.0000039943343,0.00012069366,0.00002262938,0.00013692932],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998349,0.00005145937,0.000007558453,0.00003422599,0.000022194943,0.000049698934],"domain_scores_gemma":[0.99912065,0.00037571552,0.00010156482,0.000062380655,0.00007671079,0.00026293963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049645855,0.00073478883,0.00080549275,0.00035629235,0.00068239623,0.0011679077,0.0008265033,0.000584988,0.0014219079],"category_scores_gemma":[0.0019069858,0.00027939415,0.00049396197,0.00030732556,0.0009142948,0.00051698857,0.00059406844,0.00066580606,0.00010461339],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072453724,0.0002967898,0.14368467,0.00012472564,0.00035030986,0.0003689224,0.000150256,0.8360169,0.011257922,0.0022978461,0.0011691971,0.0035578997],"study_design_scores_gemma":[0.00015788514,0.0002547521,0.06125465,0.00002563363,0.00010010812,0.000060526527,0.0001389274,0.9334336,0.0033048633,0.0006982138,0.0005260425,0.000044800887],"about_ca_topic_score_codex":0.03314254,"about_ca_topic_score_gemma":0.015980367,"teacher_disagreement_score":0.03314254,"about_ca_system_score_codex":0.0007338487,"about_ca_system_score_gemma":0.0006520138,"threshold_uncertainty_score":0.06589925},"labels":[],"label_agreement":null},{"id":"W2783894366","doi":"10.3847/1538-4357/aaab60","title":"The Next Generation Fornax Survey (NGFS). II. The Central Dwarf Galaxy Population","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Fornax Cluster; Virgo Cluster; Surface brightness; Astronomy; Galaxy; Brightest cluster galaxy; Stellar population; Stellar mass; Population; Elliptical galaxy; Star formation","score_opus":0.02478301811199494,"score_gpt":0.23681508795281608,"score_spread":0.21203206984082115,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2783894366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98794216,0.0003951947,0.00017197592,0.000054400974,0.000006696589,0.00002394587,0.0058975276,0.000032642496,0.0054754755],"genre_scores_gemma":[0.97553855,0.00022326951,0.0009564545,0.00003891081,0.000027713866,0.000044143686,0.018537566,0.00001389908,0.0046195136],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986136,0.00001688676,0.000005691441,0.00005066499,0.000031359876,0.00003401412],"domain_scores_gemma":[0.9997954,0.000013129201,0.00005873906,0.000032678032,0.00004228557,0.000057706922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028009294,0.00018874329,0.00016919783,0.001018598,0.00025962244,0.00025476582,0.0002541249,0.00010963763,0.0025531133],"category_scores_gemma":[0.00038844068,0.000059345854,0.00015375242,0.00046289118,0.00012444991,0.0003067413,0.0004244201,0.000104117775,0.0007222529],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000084872896,0.000018184686,0.97503555,0.000030525174,0.000026380303,0.000054213644,0.00029936893,0.00016923153,0.0020839383,0.000428047,0.0026296335,0.019139975],"study_design_scores_gemma":[0.000002277102,0.00001639176,0.9963924,0.0000048367983,0.0000043067894,0.00005529439,0.00006342304,0.00013340834,0.00011863568,0.000048646587,0.0031589572,0.0000013902174],"about_ca_topic_score_codex":0.020449076,"about_ca_topic_score_gemma":0.029289262,"teacher_disagreement_score":0.020449076,"about_ca_system_score_codex":0.00057871,"about_ca_system_score_gemma":0.0002626682,"threshold_uncertainty_score":0.040660083},"labels":[],"label_agreement":null},{"id":"W2784054083","doi":"10.3847/1538-4357/aaa47f","title":"CHANG-ES X: Spatially Resolved Separation of Thermal Contribution from Radio Continuum Emission in Edge-on Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Galaxy; Spectral index; Luminosity; Extinction (optical mineralogy); Calibration; Thermal; Luminous infrared galaxy; Halo","score_opus":0.007639887502205012,"score_gpt":0.23100067708986174,"score_spread":0.22336078958765673,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784054083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995907,0.000008459996,0.00016976192,0.0000031469758,3.5638027e-7,0.0000010678757,0.000048679227,0.000011064463,0.00016678846],"genre_scores_gemma":[0.9993735,0.0000046345026,0.00027452264,0.0000034107009,0.0000011956415,0.0000013153926,0.000251731,0.0000037973136,0.00008600467],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998839,0.000027467291,0.0000048646693,0.000036626247,0.000021674998,0.000025462685],"domain_scores_gemma":[0.9993356,0.00016992702,0.00015866334,0.000093342605,0.000116254516,0.00012615483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041952293,0.00022223977,0.00013032627,0.00069388613,0.00015204333,0.00038035854,0.00028410918,0.00019815266,0.0005871782],"category_scores_gemma":[0.00074112864,0.00010998726,0.00017494321,0.00042728,0.00013691005,0.00021600626,0.00035325668,0.00012861812,0.000122010664],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017865984,0.000040445433,0.97964966,0.000007405943,0.000031673313,0.000048663413,0.00009411525,0.002379122,0.011746571,0.00009210409,0.0001300429,0.005601483],"study_design_scores_gemma":[0.000005938164,0.00003454143,0.99040145,0.0000019753986,0.00001014818,0.000025774807,0.000068420275,0.006943467,0.002332493,0.000041392825,0.00013087841,0.0000034770649],"about_ca_topic_score_codex":0.0044815866,"about_ca_topic_score_gemma":0.0059218886,"teacher_disagreement_score":0.0044815866,"about_ca_system_score_codex":0.00020879747,"about_ca_system_score_gemma":0.00009775184,"threshold_uncertainty_score":0.008911014},"labels":[],"label_agreement":null},{"id":"W2784264951","doi":"10.3847/1538-4357/aaa962","title":"The Extraordinary Outburst in the Massive Protostellar System NGC 6334I-MM1: Emergence of Strong 6.7 GHz Methanol Masers","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Maser; Astrophysics; Physics; Millimeter; Excited state; Astronomy; Radiative transfer; Zeeman effect; Magnetic field; Atomic physics","score_opus":0.015072094171939622,"score_gpt":0.2641363662928112,"score_spread":0.24906427212087157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784264951","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995757,0.00003484417,0.000069243586,0.000012297327,0.0000012971699,0.0000015927855,0.000041383762,0.000011915716,0.00025181455],"genre_scores_gemma":[0.99970055,0.000017584225,0.00009829998,0.000008324368,0.0000023892328,0.0000012224917,0.000081247395,0.000001919821,0.00008843603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999454,0.0000033874423,0.0000025403308,0.000015346095,0.000016071685,0.000017219429],"domain_scores_gemma":[0.99980253,0.000009619806,0.00009135952,0.00001926676,0.000017641249,0.00005955427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099808894,0.0001700442,0.00018345227,0.00033739096,0.0004651401,0.00031923616,0.00022819142,0.00021079078,0.00057848555],"category_scores_gemma":[0.00019488337,0.000116859825,0.00012037109,0.00017934354,0.00023373435,0.0001473816,0.00056642445,0.0003617121,0.00015046321],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017051013,0.000041024923,0.71193796,0.000023036171,0.000044832297,0.0019469516,0.00048319195,0.000273676,0.278332,0.00015421459,0.0003020614,0.006290549],"study_design_scores_gemma":[0.0000022224683,0.000040483344,0.9958709,0.0000017248816,0.000006796564,0.00046698248,0.0000954417,0.00016510046,0.0029500893,0.00002726134,0.0003701545,0.0000028469424],"about_ca_topic_score_codex":0.0027458272,"about_ca_topic_score_gemma":0.0054789344,"teacher_disagreement_score":0.0027458272,"about_ca_system_score_codex":0.0002636485,"about_ca_system_score_gemma":0.000086272696,"threshold_uncertainty_score":0.0054596663},"labels":[],"label_agreement":null},{"id":"W2784342902","doi":"10.3847/1538-4357/aaaaea","title":"The Metal-poor non-Sagittarius (?) Globular Cluster NGC 5053: Orbit and Mg, Al, and Si Abundances","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Université de Franche-Comté; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Economía y Competitividad; Centre National d’Etudes Spatiales; University of Oxford; York University; Universidad Nacional Autónoma de México; Magyar Tudományos Akadémia; Space Telescope Science Institute; Sun Yat-sen University; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; National Research, Development and Innovation Office; Yale University","keywords":"Globular cluster; Observable; Spectral line; Orbit (dynamics); Star cluster; Cluster (spacecraft); Sagittarius; Hubble sequence","score_opus":0.007492305122245404,"score_gpt":0.22751467920924115,"score_spread":0.22002237408699574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784342902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994122,0.000015551675,0.000104694234,0.00001618848,0.0000016056092,0.0000016490973,0.00012465552,0.000016716605,0.00030673953],"genre_scores_gemma":[0.9996092,0.0000063770635,0.00011333472,0.000003855893,8.7493714e-7,0.0000011722699,0.00017697914,0.000003908547,0.00008431523],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999516,0.00000860337,0.0000031213976,0.000015574502,0.00000517753,0.000015991243],"domain_scores_gemma":[0.999835,0.00004323692,0.000028250142,0.000020304626,0.000022454475,0.00005071238],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013821322,0.0002518316,0.00015861732,0.00028515884,0.00028525238,0.00040837776,0.00042599053,0.0004194925,0.001303693],"category_scores_gemma":[0.00036714424,0.00013524634,0.0003187745,0.00028478092,0.0003619741,0.0002017707,0.0002567591,0.00014246744,0.00017345828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004613755,0.0001691343,0.65824026,0.00004265103,0.00018272473,0.00047752974,0.00011269395,0.32182443,0.012337238,0.0008557539,0.0012339414,0.00406231],"study_design_scores_gemma":[0.00009431317,0.00015117279,0.51964027,0.00001781622,0.00008939847,0.00010168104,0.00024734618,0.475734,0.0027255972,0.0005419321,0.00062371214,0.00003280056],"about_ca_topic_score_codex":0.049483873,"about_ca_topic_score_gemma":0.04130062,"teacher_disagreement_score":0.049483873,"about_ca_system_score_codex":0.00072701805,"about_ca_system_score_gemma":0.0002596967,"threshold_uncertainty_score":0.09839165},"labels":[],"label_agreement":null},{"id":"W2784491291","doi":"10.3847/1538-4357/aab1f3","title":"The MASSIVE Survey. IX. Photometric Analysis of 35 High-mass Early-type Galaxies with HST WFC3/IR*","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Wide Field Camera 3; Galaxy; Astronomy; Elliptical galaxy; Luminous infrared galaxy; Surface brightness; RADIUS; Effective radius; Stellar mass; Hubble space telescope; Star formation","score_opus":0.008566936934706164,"score_gpt":0.21981514988071602,"score_spread":0.21124821294600984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784491291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9887659,0.00022763516,0.00036808784,0.000034767545,0.0000033084193,0.000030103985,0.008271538,0.00010373853,0.0021948162],"genre_scores_gemma":[0.9797967,0.00015786345,0.0019407736,0.00005217186,0.000018381972,0.000027484144,0.016247155,0.000028830727,0.0017307231],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998357,0.000021263964,0.000012116236,0.000040953684,0.000039985123,0.000049976115],"domain_scores_gemma":[0.99960214,0.000015525156,0.00011908154,0.00005594258,0.000039612634,0.00016786063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041289572,0.00033195203,0.00018765978,0.0015670724,0.0003376091,0.00032842706,0.0002645479,0.00014875477,0.0016125382],"category_scores_gemma":[0.00026489949,0.00013238906,0.00027064118,0.0011778498,0.00013763677,0.0001824501,0.0005449176,0.00016517802,0.00085027877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033348938,0.00009553765,0.94926816,0.000055631997,0.00009987341,0.0002004916,0.0005270868,0.00016994242,0.016444715,0.000246867,0.00442158,0.028136628],"study_design_scores_gemma":[0.000005906243,0.00002317344,0.9980028,0.0000026335374,0.000009325301,0.000061715444,0.000030986103,0.00008035636,0.00038046847,0.00001672739,0.0013840667,0.0000018721314],"about_ca_topic_score_codex":0.009934313,"about_ca_topic_score_gemma":0.021026818,"teacher_disagreement_score":0.009934313,"about_ca_system_score_codex":0.0002873824,"about_ca_system_score_gemma":0.0001559419,"threshold_uncertainty_score":0.01975298},"labels":[],"label_agreement":null},{"id":"W2784858682","doi":"10.3847/1538-4357/aaa96d","title":"ChromaStarPy: A Stellar Atmosphere and Spectrum Modeling and Visualization Lab in Python","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Python (programming language); Java; Porting; Stellar atmosphere; Visualization; JavaScript; Scripting language; Source code","score_opus":0.010968531371500384,"score_gpt":0.271562692620127,"score_spread":0.2605941612486266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2784858682","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.005922577,0.00012658341,0.3451098,0.00044477417,0.00029461377,0.0003020831,0.013744642,0.62115365,0.012901329],"genre_scores_gemma":[0.093041986,0.0003361819,0.52417016,0.001392399,0.000261159,0.0015921043,0.051581353,0.29922393,0.028400758],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99857795,0.00018286885,0.000073586074,0.00033800447,0.0006404857,0.0001871387],"domain_scores_gemma":[0.99774843,0.0006302259,0.00014217694,0.00045766387,0.00052244274,0.0004991178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024656667,0.0014268488,0.0009630953,0.0010443635,0.00078787655,0.0023299428,0.0042973673,0.00069392944,0.060072057],"category_scores_gemma":[0.004293929,0.0010810466,0.001744492,0.00089724065,0.00090133556,0.0035496072,0.0041899863,0.0037266465,0.029066559],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017136775,0.00050730223,0.004931107,0.0009513124,0.00033356776,0.00060038187,0.0008195798,0.018022055,0.030808657,0.023236427,0.72624093,0.19183496],"study_design_scores_gemma":[0.0011349358,0.00026536526,0.005906366,0.00019345322,0.000121900775,0.00047566777,0.00017974357,0.27740517,0.0591918,0.031795125,0.6229535,0.0003770421],"about_ca_topic_score_codex":0.0032377355,"about_ca_topic_score_gemma":0.002895174,"teacher_disagreement_score":0.060072057,"about_ca_system_score_codex":0.0009074347,"about_ca_system_score_gemma":0.0027543355,"threshold_uncertainty_score":0.20096105},"labels":[],"label_agreement":null},{"id":"W2785173651","doi":"10.3847/1538-4357/aaaa72","title":"Candidate Water Vapor Lines to Locate the H<sub>2</sub>O Snowline through High-dispersion Spectroscopic Observations. III. Submillimeter H<sub>2</sub> <sup>16</sup>O and H<sub>2</sub> <sup>18</sup>O Lines","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Yukawa Institute for Theoretical Physics, Kyoto University; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Queen's University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Institutes of Natural Sciences; Japan Society for the Promotion of Science; Queen's University Belfast; University of Leeds","keywords":"Millimeter; Submillimeter Array; Snow line; Line (geometry); Water vapor; Infrared; Cosmic dust; Planet","score_opus":0.01801549498515047,"score_gpt":0.23830586858644534,"score_spread":0.22029037360129486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785173651","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99706537,0.00017806761,0.0014382118,0.000024698613,0.0000040138716,0.0000065439626,0.00012673246,0.00004508987,0.0011113355],"genre_scores_gemma":[0.9980622,0.000053923985,0.0014978613,0.0000140928405,0.0000047819512,0.0000033093677,0.00012323727,0.0000064530586,0.0002341835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999604,0.0000032975172,0.0000016027683,0.000012467935,0.0000107093465,0.000011544633],"domain_scores_gemma":[0.9998652,0.000021248032,0.0000570946,0.000009620327,0.000022372771,0.000024414529],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009767478,0.00022742403,0.00010273635,0.00042318387,0.00018121305,0.0003091531,0.00020244344,0.00026805952,0.0008863486],"category_scores_gemma":[0.00020012715,0.00013464181,0.00012306239,0.00028870057,0.000094434516,0.00036996225,0.00020119188,0.00021004805,0.00017340023],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024040836,0.000070372684,0.73512405,0.0000687081,0.00007137021,0.0002443261,0.00020838233,0.0013936723,0.23364064,0.00022834023,0.0005093915,0.028200299],"study_design_scores_gemma":[0.000027006377,0.000073106545,0.9543053,0.000018477813,0.00004875145,0.00013474272,0.0003855765,0.011889365,0.031375833,0.00020766519,0.0015231816,0.000011016164],"about_ca_topic_score_codex":0.002060143,"about_ca_topic_score_gemma":0.009680327,"teacher_disagreement_score":0.002060143,"about_ca_system_score_codex":0.000109856664,"about_ca_system_score_gemma":0.000082631246,"threshold_uncertainty_score":0.0040962696},"labels":[],"label_agreement":null},{"id":"W2785271156","doi":"10.3847/1538-4357/aaa9b9","title":"Occultations from an Active Accretion Disk in a 72-day Detached Post-Algol System Detected by K2","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Roche lobe; Eclipse; Binary star; Accretion (finance); Stars; Sky; Supernova; Orbital decay; Light curve; Orbit (dynamics)","score_opus":0.007374489455433038,"score_gpt":0.24779791071612636,"score_spread":0.24042342126069333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785271156","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988883,0.000021231383,0.000080636404,0.000013251081,0.0000028644874,0.0000039147076,0.00021608334,0.000019934008,0.000753789],"genre_scores_gemma":[0.99924576,0.00000787459,0.0001400498,0.000013347716,0.000003578862,0.0000028237412,0.00033557773,0.0000043717528,0.0002465592],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999007,0.0000050502354,0.0000065087324,0.000030981733,0.000016269993,0.000040508196],"domain_scores_gemma":[0.9997334,0.000014877588,0.000085728745,0.000033284246,0.000044483757,0.00008834705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011176888,0.00021145104,0.0001519723,0.0006045166,0.0005502643,0.0005067852,0.0002568739,0.0002643074,0.0012627286],"category_scores_gemma":[0.00023456574,0.0001354531,0.00013838452,0.00036565363,0.0001876866,0.00020481151,0.00059613417,0.00025148632,0.00040477404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030854877,0.000089164416,0.95029354,0.000023250483,0.00003424127,0.00213546,0.00036306956,0.00015558607,0.040898085,0.00008561457,0.00062470674,0.004988621],"study_design_scores_gemma":[0.0000040444843,0.000036416823,0.9962993,0.0000025718487,0.00000878637,0.00062765635,0.00015505508,0.00038537616,0.0018482608,0.000019483005,0.0006095987,0.0000033095641],"about_ca_topic_score_codex":0.005057205,"about_ca_topic_score_gemma":0.01048965,"teacher_disagreement_score":0.005057205,"about_ca_system_score_codex":0.00029718707,"about_ca_system_score_gemma":0.00013424286,"threshold_uncertainty_score":0.010055542},"labels":[],"label_agreement":null},{"id":"W2785381819","doi":"10.3847/1538-4357/aacce5","title":"A Universal Entropy Profile for the Hot Atmospheres of Galaxies and Clusters within R<sub>2500</sub>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Elliptical galaxy; Galaxy cluster; Brightest cluster galaxy; Galaxy group; Lenticular galaxy; Disc; Peculiar galaxy; Astronomy; Radio galaxy; Galaxy groups and clusters; Galaxy","score_opus":0.006503116098815515,"score_gpt":0.20246638919063584,"score_spread":0.19596327309182032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785381819","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986135,0.000059705715,0.00035956333,0.0000091147585,7.788512e-7,0.0000012284148,0.0002419138,0.000032905435,0.00068112696],"genre_scores_gemma":[0.99962115,0.000011385135,0.000086166954,0.0000022091983,9.895563e-7,7.190934e-7,0.0002142031,0.0000035696514,0.00005963854],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999654,0.000004125972,0.0000019158406,0.000009081247,0.0000073000356,0.000012161732],"domain_scores_gemma":[0.9995722,0.00010372219,0.00014043317,0.000038088365,0.00006049802,0.000084890926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001442735,0.000105163694,0.00010840127,0.0007551368,0.00014140918,0.00033007027,0.00013250753,0.00015515907,0.0008339635],"category_scores_gemma":[0.0007420014,0.00009445829,0.00017067917,0.00033194476,0.0002490591,0.0002519488,0.00022531406,0.00009727352,0.00018411396],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018468272,0.000014959706,0.93310684,0.000030086556,0.00006614105,0.00013540829,0.0003495021,0.004270347,0.05098765,0.00056362204,0.00027247472,0.010018165],"study_design_scores_gemma":[0.0000015799154,0.000022576847,0.9946622,0.000002050839,0.00000876327,0.000086547465,0.000043359763,0.0028456347,0.0018843453,0.00012989451,0.0003075487,0.000005428084],"about_ca_topic_score_codex":0.0034769203,"about_ca_topic_score_gemma":0.002864909,"teacher_disagreement_score":0.0034769203,"about_ca_system_score_codex":0.00022167705,"about_ca_system_score_gemma":0.000070101625,"threshold_uncertainty_score":0.006913364},"labels":[],"label_agreement":null},{"id":"W2785481548","doi":"10.3847/1538-4357/aaaec0","title":"Broadband Radio Polarimetry of Fornax A. I. Depolarized Patches Generated by Advected Thermal Material from NGC 1316","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Magnetic field; Polarization (electrochemistry); Polarimetry; Broadband; Faraday effect; Interstellar medium; Line-of-sight; Galaxy; Thermal","score_opus":0.005175034430346334,"score_gpt":0.19554196355566922,"score_spread":0.19036692912532288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785481548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986438,0.000053525928,0.00024033376,0.000014060821,0.0000018873171,0.000003508818,0.00018007413,0.000016401606,0.0008464535],"genre_scores_gemma":[0.998686,0.000038017308,0.0005890623,0.000014478566,0.0000072266776,0.0000036542774,0.00036796927,0.0000069358307,0.00028650905],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999466,0.000005716471,0.0000021164565,0.000019058481,0.000015131597,0.000011369622],"domain_scores_gemma":[0.9998324,0.000023588625,0.000052995456,0.000020430089,0.000033696277,0.000036791243],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108347944,0.00016638984,0.00015308111,0.00062030554,0.00022601052,0.00029660284,0.00019905857,0.00014916399,0.00068891625],"category_scores_gemma":[0.00019768634,0.00012035387,0.00013203292,0.00032189317,0.00017595752,0.00019395407,0.00033602363,0.00019157282,0.00022399097],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028998507,0.00005410331,0.2157396,0.000040120824,0.00004664949,0.0003892857,0.00040867645,0.0007182752,0.76814526,0.00013908806,0.0002563565,0.013772584],"study_design_scores_gemma":[0.000009428065,0.000054118966,0.99141276,0.000003553091,0.000013158925,0.00018575075,0.00011952972,0.00091096945,0.006686645,0.00004179071,0.00055625377,0.0000060284456],"about_ca_topic_score_codex":0.00292606,"about_ca_topic_score_gemma":0.0037045504,"teacher_disagreement_score":0.00292606,"about_ca_system_score_codex":0.00016955442,"about_ca_system_score_gemma":0.00006813371,"threshold_uncertainty_score":0.005818069},"labels":[],"label_agreement":null},{"id":"W2785700589","doi":"10.3847/1538-4357/aaac2c","title":"Herschel Spectroscopy of the Taffy Galaxies (UGC 12914/12915 = VV 254): Enhanced [C ii] Emission in the Collisionally Formed Bridge","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Spectroscopy; Emission spectrum; Star formation; Line (geometry); Spectral line; Astronomy","score_opus":0.010552088135484762,"score_gpt":0.2641458748268312,"score_spread":0.25359378669134647,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785700589","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99825174,0.00005711538,0.00022411297,0.000022503058,0.0000036503345,0.0000068831937,0.00041540895,0.00006000289,0.0009585655],"genre_scores_gemma":[0.99824834,0.000018590481,0.000608782,0.000036467052,0.0000060756165,0.000007596752,0.0007678893,0.000013581566,0.00029257548],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998549,0.000008926246,0.0000032568983,0.000049153386,0.00003862511,0.000045147855],"domain_scores_gemma":[0.9998,0.000011683467,0.0000550291,0.000026500498,0.000026389478,0.0000803879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024834726,0.00032369222,0.0003153473,0.000970717,0.00046356258,0.00031532746,0.00041510307,0.00038252192,0.0011334696],"category_scores_gemma":[0.0001739691,0.00018585875,0.00023072308,0.0005295178,0.00025505456,0.00024384564,0.00040988837,0.00030068916,0.0002988911],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027637783,0.00018479353,0.7390097,0.00004097539,0.00017582996,0.0006331983,0.00043219246,0.0010479975,0.24290451,0.00034882996,0.0019695077,0.012976177],"study_design_scores_gemma":[0.0000148950185,0.000030191755,0.995998,0.0000021951262,0.000011529225,0.00008054667,0.000032959237,0.0006182522,0.0026195354,0.000025874495,0.00056065875,0.0000053280687],"about_ca_topic_score_codex":0.010825483,"about_ca_topic_score_gemma":0.01748101,"teacher_disagreement_score":0.010825483,"about_ca_system_score_codex":0.0005565292,"about_ca_system_score_gemma":0.00019030551,"threshold_uncertainty_score":0.021524966},"labels":[],"label_agreement":null},{"id":"W2785747596","doi":"10.3847/1538-4357/aaac81","title":"The Dragonfly Nearby Galaxies Survey. IV. A Giant Stellar Disk in NGC 2841","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Surface brightness; Galaxy; Stellar mass; Astronomy; Spiral galaxy; Star formation; RADIUS; Accretion (finance); Thick disk; Stellar density; Halo","score_opus":0.00942890505645039,"score_gpt":0.22204264922976039,"score_spread":0.21261374417331,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785747596","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959126,0.00013905556,0.000039183764,0.00003958852,0.0000026370194,0.00000720215,0.002428493,0.000014711186,0.0014165877],"genre_scores_gemma":[0.9892741,0.00008844567,0.00023285893,0.000047679565,0.000006945912,0.000009841956,0.007860537,0.00000883443,0.0024708037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998449,0.000012299677,0.000008381813,0.00006286463,0.000028187447,0.00004348911],"domain_scores_gemma":[0.9996488,0.000020279538,0.0000844396,0.000028148077,0.00004967173,0.00016852148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015010983,0.00017149058,0.00019293114,0.0015767111,0.0005421516,0.00039489302,0.00026594766,0.00023351361,0.0022802674],"category_scores_gemma":[0.00023538055,0.00009645891,0.00010872322,0.0007109074,0.00015286423,0.00016378361,0.0006267211,0.00014538324,0.0007468015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000100335536,0.0000421914,0.9753509,0.000034080167,0.000025474914,0.00030448582,0.000689034,0.000102940074,0.013512804,0.000093162926,0.0017465027,0.007998173],"study_design_scores_gemma":[0.000001435289,0.000009104961,0.9987784,0.0000030735412,0.0000027687906,0.000049274116,0.00014357273,0.00003582974,0.00012138698,0.000003870904,0.000850212,9.792236e-7],"about_ca_topic_score_codex":0.05723522,"about_ca_topic_score_gemma":0.1786256,"teacher_disagreement_score":0.05723522,"about_ca_system_score_codex":0.0007427877,"about_ca_system_score_gemma":0.00021606621,"threshold_uncertainty_score":0.1138041},"labels":[],"label_agreement":null},{"id":"W2785870909","doi":"10.3847/1538-4357/aaaec4","title":"The Angular Size Distribution of μJy Radio Sources","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Full width at half maximum; Redshift; RADIUS; Angular diameter; Angular resolution (graph drawing); Galaxy; Source counts; Surface brightness; Astronomy; Brightness; Effective radius; Optics; Stars","score_opus":0.0044772411251846785,"score_gpt":0.20052224467632285,"score_spread":0.19604500355113816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2785870909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99475276,0.00032720677,0.0006815166,0.00004200254,0.0000051228208,0.0000058259193,0.0008940376,0.00006672551,0.00322484],"genre_scores_gemma":[0.99680734,0.00013204692,0.0004267939,0.00002857998,0.000029978855,0.000007539778,0.0017216058,0.000026141712,0.00082007435],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977416,0.000014201897,0.000013366867,0.00008504812,0.00006416561,0.000049085706],"domain_scores_gemma":[0.9988458,0.0001845179,0.0003842904,0.00013166857,0.00022399223,0.00022973021],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038545314,0.00015833293,0.00021814137,0.002066234,0.00025760208,0.0008128417,0.00031431238,0.00018405376,0.0034635304],"category_scores_gemma":[0.0011970294,0.0001879911,0.00016311236,0.00059684564,0.00025830546,0.00040859336,0.0005811174,0.00019407709,0.000958673],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001772785,0.0000213062,0.9393273,0.00002457709,0.000055466357,0.00014847248,0.00037150396,0.00015538532,0.04017101,0.00032857415,0.0008389707,0.018380245],"study_design_scores_gemma":[0.0000016952267,0.00000950631,0.9987515,0.0000020049963,0.0000046615382,0.000118788834,0.000027228854,0.00005910818,0.00063880073,0.00003249519,0.00035175966,0.000002368511],"about_ca_topic_score_codex":0.0017266654,"about_ca_topic_score_gemma":0.0016805585,"teacher_disagreement_score":0.0034635304,"about_ca_system_score_codex":0.0002512977,"about_ca_system_score_gemma":0.000081836326,"threshold_uncertainty_score":0.011586666},"labels":[],"label_agreement":null},{"id":"W2786160538","doi":"10.3847/1538-4357/aaafd0","title":"Advanced Diagnostics for the Study of Linearly Polarized Emission. II. Application to Diffuse Interstellar Radio Synchrotron Emission","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Polarization (electrochemistry); Faraday effect; Linear polarization; Magnetic field; Turbulence; Interstellar medium; Magnetohydrodynamics; Magnetohydrodynamic turbulence; Synchrotron","score_opus":0.010729127891325059,"score_gpt":0.29542287189215377,"score_spread":0.2846937440008287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786160538","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.071238205,0.00069670886,0.92343324,0.00023604067,0.0000754989,0.00009328091,0.00019822232,0.00083967554,0.0031890771],"genre_scores_gemma":[0.6721039,0.00046667218,0.32564,0.000076078824,0.000057727175,0.00013339179,0.0001930726,0.00009575177,0.0012334671],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989617,0.00004166911,0.0000049390997,0.0000114346385,0.00003490857,0.000010940308],"domain_scores_gemma":[0.9995184,0.00024022054,0.00009102331,0.000056471432,0.00006347909,0.000030330559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030669448,0.0004646985,0.00025346116,0.00048657673,0.00015461526,0.0003908143,0.00039172726,0.0005808574,0.0010360931],"category_scores_gemma":[0.0011744899,0.00023494556,0.00039031557,0.00048306357,0.00043456568,0.0004147965,0.00046912115,0.0007552494,0.0002072413],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009441037,0.00011293838,0.008290288,0.00014006636,0.000056212277,0.00032617874,0.00010925317,0.756163,0.09335511,0.07545294,0.0012677591,0.0646318],"study_design_scores_gemma":[0.000018774042,0.00003708483,0.0013092316,0.00000935995,0.0000036982217,0.0000851599,0.000014416912,0.9795558,0.007777152,0.009639213,0.0015375245,0.000012615783],"about_ca_topic_score_codex":0.00081519544,"about_ca_topic_score_gemma":0.0005729202,"teacher_disagreement_score":0.0010360931,"about_ca_system_score_codex":0.0003206319,"about_ca_system_score_gemma":0.0002463249,"threshold_uncertainty_score":0.0034661293},"labels":[],"label_agreement":null},{"id":"W2786189232","doi":"10.3847/1538-4357/aaac2a","title":"Discovery of Three New Millisecond Pulsars in Terzan 5","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Millisecond pulsar; Globular cluster; Pulsar; Population; Pulsar planet; Telescope; X-ray pulsar; Cluster (spacecraft)","score_opus":0.015296960622853895,"score_gpt":0.30850762401576465,"score_spread":0.29321066339291074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786189232","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986494,0.00016427801,0.00034527964,0.000014768998,0.000017635377,0.000008660852,0.00017285185,0.000016022623,0.000611154],"genre_scores_gemma":[0.99713814,0.00013753524,0.0011372223,0.000033188917,0.000023845378,0.000009361719,0.0010583579,0.00000780878,0.00045447593],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998865,0.0000054756624,0.0000057844836,0.000038198024,0.000034869765,0.000029094548],"domain_scores_gemma":[0.99974054,0.000015197238,0.00009325966,0.000030066927,0.000034072695,0.00008682532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019151565,0.00023762125,0.00034185254,0.00096785143,0.00041415085,0.0006800474,0.00024565365,0.00031439538,0.0008467457],"category_scores_gemma":[0.00030394,0.00017675036,0.00029741268,0.00073799735,0.00025559182,0.00021184699,0.0008401301,0.0004538041,0.00031864352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048789542,0.000098621946,0.8062935,0.00013034433,0.00021522942,0.0021547372,0.0008288983,0.0006255898,0.16254595,0.0007401395,0.0005655537,0.025313541],"study_design_scores_gemma":[0.000025279624,0.00021780815,0.98366433,0.000016413753,0.000074630385,0.0010581379,0.00027762738,0.00043061696,0.006291471,0.00020481016,0.0077228895,0.000015915539],"about_ca_topic_score_codex":0.0008963533,"about_ca_topic_score_gemma":0.0016869876,"teacher_disagreement_score":0.00096785143,"about_ca_system_score_codex":0.00023704626,"about_ca_system_score_gemma":0.0001425812,"threshold_uncertainty_score":0.0028326511},"labels":[],"label_agreement":null},{"id":"W2786208944","doi":"10.3847/1538-4357/aaadad","title":"The Properties of Planck Galactic Cold Clumps in the L1495 Dark Cloud","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Planck; Molecular cloud; Star formation; Galaxy; Stars","score_opus":0.015264746416779352,"score_gpt":0.23368397712240574,"score_spread":0.21841923070562638,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786208944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990503,0.000054256892,0.000117265095,0.000011931007,0.0000018751527,0.0000030763813,0.00034619577,0.000008227603,0.0004068908],"genre_scores_gemma":[0.9993789,0.00001277393,0.00008005497,0.000007692862,0.000002083587,0.0000020063687,0.0004181211,0.0000030109052,0.000095288924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999291,0.0000036612903,0.0000036149304,0.000024242976,0.000015031044,0.000024456425],"domain_scores_gemma":[0.99968314,0.000038598664,0.000075113385,0.000038665792,0.000039362734,0.00012520743],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013840116,0.00014343442,0.00017874534,0.00053279806,0.00038991525,0.00039082958,0.00025218408,0.00016231365,0.0012080283],"category_scores_gemma":[0.00044402832,0.000112830836,0.00013382813,0.00038112383,0.00029206704,0.00020855911,0.00046829303,0.00015409719,0.00018717226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025883314,0.000035033,0.94712067,0.00003204879,0.000070527945,0.00033500197,0.0003167059,0.0022894987,0.043370374,0.00040585292,0.00085077033,0.004914637],"study_design_scores_gemma":[0.000011230234,0.000025967736,0.9937797,0.000004420748,0.00001110986,0.000061997096,0.00014319326,0.0027870703,0.0024541933,0.0001288929,0.0005851164,0.000007021912],"about_ca_topic_score_codex":0.012441589,"about_ca_topic_score_gemma":0.008198492,"teacher_disagreement_score":0.012441589,"about_ca_system_score_codex":0.00048393136,"about_ca_system_score_gemma":0.00010504663,"threshold_uncertainty_score":0.024738312},"labels":[],"label_agreement":null},{"id":"W2786803886","doi":"10.3847/1538-4357/aaae09","title":"BANYAN. XI. The BANYAN Σ Multivariate Bayesian Algorithm to Identify Members of Young Associations with 150 pc","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":509,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Multivariate statistics; Bayesian probability; Sky; Gaussian; Field (mathematics); Multivariate analysis; Parallax; Stars","score_opus":0.011009775299612789,"score_gpt":0.2605669152269326,"score_spread":0.24955713992731982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786803886","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.020066073,0.0006354044,0.9533249,0.00032276125,0.00012979281,0.0002367065,0.0018029858,0.015373218,0.008108126],"genre_scores_gemma":[0.08696246,0.00027280967,0.8926658,0.00041726168,0.00010101692,0.00036942138,0.0060510817,0.0020140295,0.011146064],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992073,0.00019068267,0.0000487377,0.00023425395,0.00022278418,0.00009633559],"domain_scores_gemma":[0.99898833,0.00037433754,0.0001052049,0.00016783115,0.0002836853,0.00008062264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017852274,0.00093957456,0.0010365547,0.001973934,0.0011380343,0.0016181676,0.001929268,0.00096193474,0.011631447],"category_scores_gemma":[0.0052567585,0.00070664426,0.0010522342,0.0011889848,0.00047047355,0.0013434042,0.002755246,0.0014291886,0.0077650137],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005697465,0.000110049594,0.013606437,0.00022889019,0.00032888784,0.00010551378,0.0002472619,0.06366985,0.006286736,0.020466227,0.036876615,0.8575039],"study_design_scores_gemma":[0.00014748525,0.00008985352,0.0050041177,0.00010895704,0.00007809872,0.00028066259,0.00014938282,0.89515704,0.011076125,0.042037938,0.04580945,0.000060922146],"about_ca_topic_score_codex":0.010985523,"about_ca_topic_score_gemma":0.0103717195,"teacher_disagreement_score":0.011631447,"about_ca_system_score_codex":0.00085265154,"about_ca_system_score_gemma":0.001970952,"threshold_uncertainty_score":0.038911104},"labels":[],"label_agreement":null},{"id":"W2786831769","doi":"10.3847/1538-4357/aaad09","title":"Seeds of Life in Space (SOLIS). III. Zooming Into the Methanol Peak of the Prestellar Core L1544*","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Radiative transfer; Methanol; Astrochemistry; Kinematics; Mean kinetic temperature; Hydrogen; Core (optical fiber); Space (punctuation)","score_opus":0.013764198519605938,"score_gpt":0.2520141822559181,"score_spread":0.23824998373631215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2786831769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99394256,0.000074287316,0.00062877376,0.00004828015,0.000009086127,0.000012046625,0.000716528,0.00025246092,0.0043159034],"genre_scores_gemma":[0.9970721,0.000023853258,0.0010553725,0.0000114298655,0.000004038842,0.0000071309414,0.00095171074,0.000039394192,0.0008350491],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999776,0.0000025305376,4.520247e-7,0.000005873551,0.0000059274817,0.00000762676],"domain_scores_gemma":[0.9999287,0.000009868582,0.000014638845,0.0000063373714,0.0000066285747,0.000033721542],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059574646,0.00023328685,0.00008965001,0.00036722896,0.00023893073,0.00020094535,0.00013217489,0.0001250349,0.002114029],"category_scores_gemma":[0.00010732776,0.000097393626,0.00016790871,0.0001713059,0.00012560791,0.00014614589,0.00029460274,0.00016102569,0.00024142263],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025758857,0.00035153393,0.26419264,0.00022193012,0.00021389553,0.0022908829,0.0014589721,0.017387936,0.5778729,0.0022494267,0.009625308,0.12155875],"study_design_scores_gemma":[0.00005713918,0.00046160963,0.90812385,0.000015707235,0.000027697686,0.00040929785,0.00048077272,0.024387829,0.052062944,0.00070584216,0.013242849,0.00002440646],"about_ca_topic_score_codex":0.0029291764,"about_ca_topic_score_gemma":0.007667257,"teacher_disagreement_score":0.0029291764,"about_ca_system_score_codex":0.00029102527,"about_ca_system_score_gemma":0.00008037061,"threshold_uncertainty_score":0.0070721507},"labels":[],"label_agreement":null},{"id":"W2787075170","doi":"10.3847/1538-4357/aab043","title":"The Next Generation Virgo Cluster Survey (NGVS). XVIII. Measurement and Calibration of Surface Brightness Fluctuation Distances for Bright Galaxies in Virgo (and Beyond)","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Virgo Cluster; Astrophysics; Galaxy; Photometry (optics); Surface brightness; Calibration; Astronomy; Stellar population; Brightness; Galaxy cluster; Star formation; Stars","score_opus":0.025776178670815785,"score_gpt":0.23303710791771173,"score_spread":0.20726092924689596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787075170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8364968,0.0006974705,0.010513613,0.00020960724,0.00006371589,0.00071138766,0.13318297,0.0023080702,0.015816355],"genre_scores_gemma":[0.6965013,0.00026910668,0.044365335,0.00017906379,0.000050175036,0.0006825117,0.24941498,0.000264403,0.008273239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968743,0.000045364875,0.000014992927,0.00007057659,0.00012476061,0.000056809542],"domain_scores_gemma":[0.99927086,0.000047201214,0.00015214624,0.0001626093,0.00019365162,0.00017351189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006896483,0.00030636135,0.000230183,0.0021015822,0.00034433135,0.00039027596,0.0005965687,0.0001906804,0.0015623166],"category_scores_gemma":[0.0009478963,0.00017411198,0.0002114599,0.0015936284,0.00012880492,0.0001931196,0.0005768759,0.0002096395,0.0009939455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024345552,0.00010093534,0.84172344,0.00012449357,0.00014786205,0.00009384784,0.00029930592,0.0019328338,0.0123475185,0.0011291449,0.040569883,0.101287335],"study_design_scores_gemma":[0.000017730457,0.000028344648,0.97874475,0.000010694419,0.000016324422,0.000045101082,0.000040566418,0.0015309141,0.0019899379,0.00013841609,0.017427497,0.000009771381],"about_ca_topic_score_codex":0.049174633,"about_ca_topic_score_gemma":0.0758036,"teacher_disagreement_score":0.049174633,"about_ca_system_score_codex":0.0008589567,"about_ca_system_score_gemma":0.0007090292,"threshold_uncertainty_score":0.09777683},"labels":[],"label_agreement":null},{"id":"W2787081012","doi":"10.3847/1538-4357/aaadb1","title":"The MAVERIC Survey: A Red Straggler Binary with an Invisible Companion in the Galactic Globular Cluster M10","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; White dwarf; Neutron star; Star cluster; Black hole (networking); Red giant; Galaxy; Active galactic nucleus; Accretion (finance)","score_opus":0.020712296295104488,"score_gpt":0.25320358885268746,"score_spread":0.23249129255758297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787081012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991296,0.00007926266,0.000024227382,0.000021603588,0.0000021585743,0.0000022918377,0.00007390318,0.000004559824,0.0006624519],"genre_scores_gemma":[0.9992524,0.000054572665,0.000057973863,0.000030113642,0.0000053921417,0.0000014521432,0.00024732412,0.0000020143966,0.0003488272],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999859,0.000014294076,0.0000062676195,0.00003915242,0.00003074697,0.000050539013],"domain_scores_gemma":[0.9997129,0.000021416281,0.00007446847,0.000021598542,0.00003307747,0.00013642809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016405995,0.00023475142,0.0001594489,0.0009990176,0.00060749927,0.0005062787,0.0004194483,0.00027388666,0.0009191599],"category_scores_gemma":[0.00024517608,0.00010234015,0.00010941423,0.0004968743,0.0003740842,0.00017317718,0.0005559074,0.00018936806,0.00035422997],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014945917,0.00006315584,0.9834667,0.00001251664,0.000019546773,0.0010956441,0.0005305763,0.000046751757,0.008905107,0.00017541434,0.00056128466,0.004973719],"study_design_scores_gemma":[0.000007659297,0.00011084203,0.9950724,0.0000071238105,0.000012584861,0.001398604,0.0006649307,0.00015642088,0.0005943922,0.000037124595,0.0019345827,0.00000333169],"about_ca_topic_score_codex":0.0206342,"about_ca_topic_score_gemma":0.03961899,"teacher_disagreement_score":0.0206342,"about_ca_system_score_codex":0.00074743904,"about_ca_system_score_gemma":0.00027090163,"threshold_uncertainty_score":0.0410282},"labels":[],"label_agreement":null},{"id":"W2787255625","doi":"10.3847/1538-4357/aab6b5","title":"Superresolution Interferometric Imaging with Sparse Modeling Using Total Squared Variation: Application to Imaging the Black Hole Shadow","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Supermassive black hole; Point spread function; Interferometry; Iterative reconstruction; Gaussian; Brightness; Image resolution; Shadow (psychology); Regularization (linguistics); RADIUS","score_opus":0.017129108783035717,"score_gpt":0.24411456917841065,"score_spread":0.22698546039537493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787255625","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.16223553,0.00015612472,0.83621126,0.00026106526,0.000016737768,0.000017833769,0.000043480388,0.00031982758,0.00073820463],"genre_scores_gemma":[0.80529064,0.00010103013,0.19414093,0.00004673736,0.000023097231,0.000013796211,0.000081409715,0.000037585123,0.00026462539],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998636,0.00004636977,0.0000048326883,0.000019595043,0.000050501378,0.000014991323],"domain_scores_gemma":[0.99973565,0.00010118519,0.00004941965,0.00004912901,0.000041807332,0.000022719461],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000513883,0.00039226626,0.0003597814,0.00038428532,0.00015314331,0.000339377,0.00044377564,0.00032693785,0.0002588787],"category_scores_gemma":[0.000900321,0.00019829119,0.0004062893,0.00041827263,0.00042598753,0.00042184506,0.0005260161,0.00040297088,0.000051501607],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015949452,0.00006667198,0.003756395,0.000059269605,0.000093223636,0.00019695847,0.000104787665,0.8280042,0.10208465,0.009242282,0.0006299155,0.05560212],"study_design_scores_gemma":[0.0000028155534,0.000010075483,0.00034387474,6.9329747e-7,0.0000018621956,0.0000135788905,0.0000039325128,0.99703085,0.0019013652,0.00059508573,0.00009243813,0.0000033647857],"about_ca_topic_score_codex":0.0020116388,"about_ca_topic_score_gemma":0.0015825401,"teacher_disagreement_score":0.0020116388,"about_ca_system_score_codex":0.00022808809,"about_ca_system_score_gemma":0.00027662065,"threshold_uncertainty_score":0.003999889},"labels":[],"label_agreement":null},{"id":"W2787350953","doi":"10.3847/1538-4357/aaae06","title":"Polycyclic Aromatic Hydrocarbon Emission Toward the Galactic Bulge","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Astrophysics; Physics; Bulge; Polycyclic aromatic hydrocarbon; Outflow; Population; Extinction (optical mineralogy); Astronomy; Molecular cloud; Galaxy; Astrobiology; Stars","score_opus":0.012616740740998965,"score_gpt":0.24840269932916148,"score_spread":0.2357859585881625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787350953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994438,0.000034543307,0.000027547572,0.000005926736,8.0055736e-7,0.0000013059254,0.0001731744,0.000006863388,0.00030599834],"genre_scores_gemma":[0.99922276,0.000029030405,0.00008104609,0.00001663493,0.0000025707434,0.000002089631,0.0005035003,0.0000018088939,0.00014056038],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995184,0.0000026919222,0.0000013881775,0.000014047988,0.00000952024,0.000020455476],"domain_scores_gemma":[0.9998307,0.000011827053,0.000048335736,0.000011361433,0.000031029154,0.00006673844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007049036,0.00023911144,0.00013466325,0.0008222927,0.00022588753,0.00030518798,0.00012889867,0.00015319383,0.00072455365],"category_scores_gemma":[0.00012105066,0.00009571555,0.00012804213,0.00042170996,0.00015516083,0.00012630115,0.0002399688,0.00012268628,0.00016289989],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018694173,0.000037701215,0.92964655,0.000023716259,0.000067709494,0.00017809242,0.0001927356,0.0005222441,0.06245714,0.000046362362,0.00045667004,0.006184122],"study_design_scores_gemma":[0.0000013234701,0.000012835007,0.9991098,0.0000015418254,0.0000034395443,0.00002689839,0.00003803986,0.00011084223,0.0005702712,0.0000036465938,0.00012040499,9.4361417e-7],"about_ca_topic_score_codex":0.020026525,"about_ca_topic_score_gemma":0.027351137,"teacher_disagreement_score":0.020026525,"about_ca_system_score_codex":0.00039008012,"about_ca_system_score_gemma":0.00008751042,"threshold_uncertainty_score":0.039819956},"labels":[],"label_agreement":null},{"id":"W2787385412","doi":"10.3847/1538-4357/aaabb7","title":"The Strong Gravitationally Lensed Herschel Galaxy HLock01: Optical Spectroscopy Reveals a Close Galaxy Merger with Evidence of Inflowing Gas","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; National Key Research and Development Program of China; Science and Technology Facilities Council; Office of Science; Centre National de la Recherche Scientifique; U.S. Department of Energy; National Natural Science Foundation of China; Cardiff University; York University; Ohio State University; UK Space Agency; Instituto de Astrofísica de Canarias; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Harvard University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Imperial College London; National Science Foundation; California Institute of Technology; National Aeronautics and Space Administration; Centre National d’Etudes Spatiales","keywords":"Galaxy; Redshift; Spectroscopy; Stars; Star formation; Active galactic nucleus; Galaxy merger; Gravitational lens","score_opus":0.011643591840041012,"score_gpt":0.2537269021114546,"score_spread":0.24208331027141358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787385412","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989768,0.00007524372,0.00006505506,0.000022477265,0.0000016312862,0.0000024808355,0.00012369736,0.0000140358425,0.0007185241],"genre_scores_gemma":[0.99956685,0.000013101087,0.00009523207,0.000022002421,0.0000030076887,9.755265e-7,0.00017840286,0.0000023492137,0.00011817456],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998858,0.0000069914354,0.000005000019,0.00003231808,0.000027549533,0.000042337335],"domain_scores_gemma":[0.99976176,0.000015884558,0.000084963474,0.000021027688,0.000017864497,0.000098438555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013448078,0.00018857168,0.00021505683,0.0007310476,0.00031827646,0.0005278629,0.00028211746,0.00031365204,0.0012730949],"category_scores_gemma":[0.00016688001,0.00013716094,0.00011023464,0.000420098,0.00029357764,0.00022073301,0.0005619207,0.00021010374,0.00033752428],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022576601,0.00011691048,0.79691297,0.000024336849,0.00008194947,0.0021417437,0.0003939264,0.00025888818,0.19200051,0.00040506633,0.000798108,0.006639807],"study_design_scores_gemma":[0.000009101297,0.00004528254,0.9955224,0.000002700276,0.000012611605,0.0008259763,0.00018701839,0.00039911276,0.0023315225,0.000041765794,0.00061811105,0.000004533398],"about_ca_topic_score_codex":0.0046209455,"about_ca_topic_score_gemma":0.007427951,"teacher_disagreement_score":0.0046209455,"about_ca_system_score_codex":0.0003906137,"about_ca_system_score_gemma":0.00009883649,"threshold_uncertainty_score":0.009188056},"labels":[],"label_agreement":null},{"id":"W2787521172","doi":"10.3847/1538-4357/aab040","title":"High-redshift Extremely Red Quasars in X-Rays","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Johns Hopkins University; Smithsonian Institution","keywords":"Quasar; Luminosity; Infrared; Accretion (finance); Star formation; Accretion disc; Absorption (acoustics); Red shift","score_opus":0.010736030288235221,"score_gpt":0.21999344690303502,"score_spread":0.2092574166147998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787521172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99854857,0.000109850174,0.00021059786,0.00002062402,0.0000018843712,0.0000015712276,0.00006209465,0.000016027927,0.0010286685],"genre_scores_gemma":[0.9994085,0.000037423273,0.00012025161,0.000024927753,0.000006716275,8.337485e-7,0.0000759869,0.0000018278006,0.00032354682],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985874,0.000014851993,0.0000090567455,0.00003692741,0.000036405483,0.000044023425],"domain_scores_gemma":[0.9993387,0.00008722239,0.00036358074,0.000059736314,0.00006411724,0.000086648004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028661653,0.00024901924,0.00021185141,0.0006854861,0.00029253884,0.00073425303,0.000241282,0.00024509567,0.0021459393],"category_scores_gemma":[0.00036852199,0.00014806165,0.00013318054,0.00032993214,0.0003546802,0.0003639799,0.0004470691,0.00025711133,0.00032822954],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046783098,0.000031575335,0.971108,0.000018874645,0.00003739554,0.0002800969,0.00022392927,0.00015729507,0.02211613,0.00031733752,0.00013594385,0.0055267215],"study_design_scores_gemma":[0.0000010054409,0.00001691644,0.9984211,0.0000027094763,0.000006850678,0.00025673903,0.00009347828,0.000084853426,0.00071621645,0.000061653234,0.0003370964,0.0000013807132],"about_ca_topic_score_codex":0.0007908914,"about_ca_topic_score_gemma":0.0014689876,"teacher_disagreement_score":0.0021459393,"about_ca_system_score_codex":0.00010694915,"about_ca_system_score_gemma":0.00004627102,"threshold_uncertainty_score":0.0071789026},"labels":[],"label_agreement":null},{"id":"W2787688820","doi":"10.3847/1538-4357/aaaf65","title":"A UV-to-NIR Study of Molecular Gas in the Dust Cavity around RY Lupi","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Astrophysics; Gaussian; Physics; Component (thermodynamics); Flux (metallurgy); Line (geometry); Spectral line; Emission spectrum; Gaussian network model; Chemistry; Geometry; Astronomy; Mathematics","score_opus":0.013067338014495927,"score_gpt":0.26468077684876606,"score_spread":0.2516134388342701,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787688820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987753,0.00007564212,0.00027394207,0.00001276781,0.0000010026869,0.000004429441,0.000074526804,0.000028524544,0.0007538758],"genre_scores_gemma":[0.99940455,0.000031744214,0.00030780386,0.000007622753,0.0000036326587,0.0000034048887,0.00010242897,0.000006225991,0.0001326832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996996,0.0000037192272,8.5708393e-7,0.0000092187565,0.000005700316,0.000010536127],"domain_scores_gemma":[0.99991596,0.00001723931,0.00001903759,0.000007621564,0.000011974017,0.000028235674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000098019074,0.00016987968,0.00019756913,0.00043044752,0.00036178264,0.00025990975,0.0002887603,0.00018031918,0.000739432],"category_scores_gemma":[0.00016116686,0.00012312942,0.00020020235,0.00020135577,0.00016532914,0.0001919881,0.00025462353,0.00015837883,0.00020252433],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006616027,0.00029310523,0.50198704,0.00011004209,0.00014198711,0.0018251555,0.00089677656,0.012718088,0.46343058,0.00079216977,0.00048101397,0.01666231],"study_design_scores_gemma":[0.00002860059,0.00019582681,0.97294015,0.000009311429,0.00004489697,0.000288092,0.0002805903,0.018264916,0.006975695,0.00015347816,0.000808142,0.00001031161],"about_ca_topic_score_codex":0.0049709077,"about_ca_topic_score_gemma":0.0036379737,"teacher_disagreement_score":0.0049709077,"about_ca_system_score_codex":0.00029683395,"about_ca_system_score_gemma":0.00012257414,"threshold_uncertainty_score":0.00988394},"labels":[],"label_agreement":null},{"id":"W2787925641","doi":"10.3847/1538-4357/aabd87","title":"OGLE-2017-BLG-0329L: A Microlensing Binary Characterized with Dramatically Enhanced Precision Using Data from Space-based Observations","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Jet Propulsion Laboratory; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Korea Research Environment Open Network; National Research Foundation of Korea; Korea Institute of Science and Technology Information; Universities Space Research Association; Iran National Science Foundation; Science and Technology Facilities Council; National Research Foundation; Korea Institute of Science and Technology; Narodowym Centrum Nauki; National Science Foundation","keywords":"Gravitational microlensing; Parallax; Microlens; Einstein radius; Binary number; Caustic (mathematics); Degeneracy (biology); Occultation; Gravitational lens","score_opus":0.06517564416765818,"score_gpt":0.3466132437315843,"score_spread":0.2814375995639261,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2787925641","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936486,0.00014718976,0.0018878166,0.00014097481,0.000017413486,0.000014138782,0.0011569578,0.0001534694,0.0028333322],"genre_scores_gemma":[0.99511623,0.0000318488,0.0018946724,0.000072567585,0.000015081182,0.000007075766,0.0025235643,0.00004896122,0.00028994415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995732,0.000036651378,0.000022119855,0.00014922739,0.00013155953,0.00008721366],"domain_scores_gemma":[0.998638,0.00017551545,0.00062660646,0.00019492838,0.00013734217,0.00022755968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077378744,0.00037384106,0.0005818429,0.0013135481,0.000620221,0.0018012157,0.00038377862,0.00054193026,0.0010371775],"category_scores_gemma":[0.0011967311,0.0001944125,0.00031541134,0.0012542234,0.00038629147,0.00042214835,0.00093599386,0.00072290114,0.0005268395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009366422,0.0003091843,0.8467686,0.00011906416,0.000318617,0.0021038835,0.00038583556,0.006331379,0.1042825,0.0069083422,0.002942484,0.028593432],"study_design_scores_gemma":[0.00014986517,0.00013614209,0.9386879,0.000029735926,0.000093473565,0.0011747173,0.00029270348,0.034046873,0.015359964,0.0027893134,0.0071708467,0.000068467125],"about_ca_topic_score_codex":0.0035274774,"about_ca_topic_score_gemma":0.005994017,"teacher_disagreement_score":0.0035274774,"about_ca_system_score_codex":0.0008914813,"about_ca_system_score_gemma":0.00033344878,"threshold_uncertainty_score":0.0070138574},"labels":[],"label_agreement":null},{"id":"W2788039407","doi":"10.3847/1538-4357/aab03e","title":"Hubble Space Telescope Observations of Extended [O iii]λ 5007 Emission in Nearby QSO2s: New Constraints on AGN Host Galaxy Interaction","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Lawrence Berkeley National Laboratory; Office of Naval Research; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; University of Oxford; York University; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Universities Space Research Association; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Goddard Space Flight Center; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Danmarks Frie Forskningsfond; National Science Foundation","keywords":"Galaxy; Bulge; Active galactic nucleus; Hubble space telescope; Luminosity; Quasar; RADIUS; Doubly ionized oxygen; Star formation","score_opus":0.01750257644329117,"score_gpt":0.2533511305580844,"score_spread":0.23584855411479322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788039407","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985942,0.00007341308,0.00019870362,0.000010059151,9.627786e-7,0.0000024181363,0.00017598107,0.000013271206,0.0009308728],"genre_scores_gemma":[0.9993748,0.000034730023,0.00013918213,0.000013913242,0.0000059309627,0.0000021302228,0.00030113754,0.000003245879,0.00012502182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999889,0.000011802908,0.0000055813102,0.000029638852,0.000029129686,0.000034877772],"domain_scores_gemma":[0.999388,0.0000735219,0.00020417552,0.00006757902,0.000063593754,0.0002030425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027306977,0.00027580268,0.0002545534,0.00095787324,0.00026806208,0.0006450766,0.00022680343,0.00027863655,0.0016083001],"category_scores_gemma":[0.0004865484,0.0001556595,0.00017843234,0.00056688034,0.00031025565,0.00042145493,0.000475582,0.00017239986,0.00033310216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010584516,0.00004483168,0.9593426,0.00002005603,0.000062635925,0.00015985464,0.00027336474,0.0002818637,0.035969503,0.0001848019,0.00020274929,0.0033518798],"study_design_scores_gemma":[0.0000022851113,0.000013284691,0.99910295,0.0000024267326,0.000007077247,0.000044847173,0.00006023318,0.00017123608,0.00037838504,0.000037794358,0.00017758878,0.0000018893917],"about_ca_topic_score_codex":0.004571247,"about_ca_topic_score_gemma":0.010939712,"teacher_disagreement_score":0.004571247,"about_ca_system_score_codex":0.00027923062,"about_ca_system_score_gemma":0.000108831104,"threshold_uncertainty_score":0.009089291},"labels":[],"label_agreement":null},{"id":"W2788137830","doi":"10.3847/1538-4357/aabf3f","title":"OGLE-2016-BLG-1266: A Probable Brown Dwarf/Planet Binary at the Deuterium Fusion Limit","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Binary number; Parallax; Brown dwarf; Binary star; Measure (data warehouse); Telescope; Limit (mathematics); Deuterium","score_opus":0.013174493911474199,"score_gpt":0.21953638472799836,"score_spread":0.20636189081652415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788137830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99345446,0.00021365515,0.0011014721,0.000337451,0.000021888241,0.000007814115,0.0002626833,0.00008612171,0.004514347],"genre_scores_gemma":[0.9989373,0.000011459802,0.00029574052,0.00008235618,0.00000960025,7.761914e-7,0.00012720987,0.0000065528297,0.00052900444],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998282,0.000015925127,0.000011102135,0.000055791967,0.000041413645,0.000047557387],"domain_scores_gemma":[0.9994271,0.00006563002,0.00017455283,0.000062644256,0.00005628085,0.0002139233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041107088,0.00026707764,0.00047451377,0.0007592291,0.0012647905,0.0012235454,0.00038522648,0.0011729443,0.003170902],"category_scores_gemma":[0.0006318459,0.00017489702,0.00016701022,0.00043250632,0.00064749294,0.00040606046,0.00068312365,0.00055131165,0.0014129766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016670616,0.00049540476,0.7936386,0.00013851507,0.000090987705,0.0252679,0.0006781985,0.0021891461,0.12946722,0.012599168,0.003709025,0.030058792],"study_design_scores_gemma":[0.00022799699,0.0011891229,0.8217573,0.000067151275,0.00010515657,0.05617033,0.0012595903,0.025262194,0.052780323,0.02081291,0.020250313,0.00011763598],"about_ca_topic_score_codex":0.0012770669,"about_ca_topic_score_gemma":0.0016294693,"teacher_disagreement_score":0.003170902,"about_ca_system_score_codex":0.00061688485,"about_ca_system_score_gemma":0.00017889777,"threshold_uncertainty_score":0.010607719},"labels":[],"label_agreement":null},{"id":"W2788357060","doi":"10.3847/1538-4357/aabcd2","title":"OGLE-2017-BLG-1130: The First Binary Gravitational Microlens Detected from Spitzer Only","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; National Research Foundation of Korea; National Natural Science Foundation of China; Jet Propulsion Laboratory; National Research Foundation; California Institute of Technology; National Aeronautics and Space Administration; Universities Space Research Association; Narodowym Centrum Nauki; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Gravitational microlensing; Degeneracy (biology); Binary number; Parallax; Event (particle physics); Light curve; Microlens; Anomaly (physics)","score_opus":0.010811210597800347,"score_gpt":0.22337878380175313,"score_spread":0.21256757320395278,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788357060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949838,0.00013518168,0.0010134778,0.00009491266,0.00002392985,0.000012555366,0.0008447905,0.00011654434,0.0027748116],"genre_scores_gemma":[0.99724907,0.000026944665,0.000554427,0.00004410876,0.000020484116,0.0000035173196,0.0017392213,0.00003387627,0.00032840285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99952614,0.000025112495,0.000021982652,0.00009903544,0.00016011788,0.00016760826],"domain_scores_gemma":[0.99867696,0.00020732668,0.00041954016,0.00020955924,0.00015408709,0.00033258856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005317138,0.0003587265,0.00054283236,0.0018919584,0.00084525073,0.0013939722,0.00033237637,0.00059715664,0.0015901922],"category_scores_gemma":[0.0015535842,0.00016225438,0.00040292938,0.0010498106,0.00068456883,0.00044123444,0.001650821,0.0006853492,0.0006551953],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094907626,0.00023492116,0.9268034,0.00011577187,0.00022856538,0.007559937,0.00073051616,0.001073734,0.027334727,0.003813341,0.0033718476,0.027784178],"study_design_scores_gemma":[0.000045872166,0.00020503675,0.9650787,0.00003355602,0.00009044743,0.005295661,0.0004994031,0.004310313,0.011864258,0.0019661568,0.010558318,0.000052322303],"about_ca_topic_score_codex":0.0047758864,"about_ca_topic_score_gemma":0.006221914,"teacher_disagreement_score":0.0047758864,"about_ca_system_score_codex":0.0009850984,"about_ca_system_score_gemma":0.00041231123,"threshold_uncertainty_score":0.009496152},"labels":[],"label_agreement":null},{"id":"W2788491848","doi":"10.3847/1538-4357/aab0a6","title":"Stellar Populations of over 1000 z ∼ 0.8 Galaxies from LEGA-C: Ages and Star Formation Histories from D<sub>n</sub>4000 and Hδ","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Elliptical galaxy; Lenticular galaxy; Stellar population; Peculiar galaxy; Star formation; Surface brightness fluctuation; Luminous infrared galaxy; Galaxy group","score_opus":0.009308031152807381,"score_gpt":0.2075838625179623,"score_spread":0.19827583136515492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788491848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955344,0.00008759465,0.000074437165,0.000027149661,0.0000019716165,0.00000541569,0.003549922,0.000020627192,0.00069843634],"genre_scores_gemma":[0.9902125,0.000038654576,0.0002714798,0.000041537318,0.0000076892475,0.00000798355,0.009134286,0.0000114387985,0.00027446443],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975556,0.00003569861,0.00001495415,0.00008046071,0.000048629485,0.000064709435],"domain_scores_gemma":[0.99878246,0.00020416432,0.0003444877,0.0001396535,0.00017004788,0.00035919968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039186561,0.00030334308,0.0002548941,0.0024032681,0.00039151293,0.0010197967,0.00046672233,0.0005109712,0.0010441546],"category_scores_gemma":[0.0008798452,0.00016077913,0.0002802687,0.0014365133,0.0003091505,0.00033686575,0.0007428897,0.0002535199,0.0005996836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001754814,0.000046311714,0.9894666,0.000018511713,0.00009569343,0.00008703228,0.00028343566,0.00033172622,0.0038160537,0.00009861598,0.0007857884,0.0047947075],"study_design_scores_gemma":[0.0000055054597,0.00001585549,0.9988121,0.0000037787588,0.0000105704175,0.00005155013,0.00007111985,0.00031453374,0.00021894553,0.00002156392,0.00047070268,0.00000380982],"about_ca_topic_score_codex":0.016762573,"about_ca_topic_score_gemma":0.025133569,"teacher_disagreement_score":0.016762573,"about_ca_system_score_codex":0.00062564627,"about_ca_system_score_gemma":0.00012977666,"threshold_uncertainty_score":0.033330023},"labels":[],"label_agreement":null},{"id":"W2788518763","doi":"10.3847/1538-4357/aac6d5","title":"About 30% of Sun-like Stars Have Kepler-like Planetary Systems: A Study of Their Intrinsic Architecture","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":259,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planet; Physics; Planetary system; Kepler; Astrophysics; Stars; Kepler-47; Astronomy; Orbital elements; Planetary migration","score_opus":0.012012970331349054,"score_gpt":0.22339248618782231,"score_spread":0.21137951585647327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788518763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99932694,0.000040433402,0.00017828522,0.000013889442,3.0167885e-7,6.597799e-7,0.0000765935,0.0000033534905,0.0003594183],"genre_scores_gemma":[0.99968696,0.000026227637,0.00012289204,0.0000022036916,9.738905e-7,6.141653e-7,0.00010277058,0.0000013998714,0.000055981538],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987686,0.000023060786,0.000008922782,0.00005052035,0.00001845695,0.000022148173],"domain_scores_gemma":[0.9991792,0.0002207973,0.0002771535,0.00012476798,0.00007237362,0.00012561996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032462025,0.00014384477,0.00019554395,0.0005796678,0.00027666072,0.0006657674,0.00027431053,0.000216879,0.0017539063],"category_scores_gemma":[0.0013912752,0.00017076952,0.00025412708,0.0005537038,0.00027050983,0.0007579582,0.00046442528,0.00016239553,0.00037176482],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056585042,0.000011902285,0.9914096,0.000007842107,0.000043501765,0.000034717476,0.000099375975,0.002016103,0.0023529564,0.0005058621,0.000059168997,0.003402352],"study_design_scores_gemma":[0.000002334278,0.00003316155,0.99023646,0.000003536388,0.000016265865,0.00019730137,0.00011168534,0.008039742,0.0005340162,0.00053099834,0.00029067576,0.000003975056],"about_ca_topic_score_codex":0.0011659403,"about_ca_topic_score_gemma":0.002139404,"teacher_disagreement_score":0.0017539063,"about_ca_system_score_codex":0.00018183806,"about_ca_system_score_gemma":0.000112669884,"threshold_uncertainty_score":0.005867362},"labels":[],"label_agreement":null},{"id":"W2788675381","doi":"10.3847/1538-4357/aaae63","title":"The Next Generation Virgo Cluster Survey (NGVS). XXXII. A Search for Globular Cluster Substructures in the Virgo Galaxy Cluster Core","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Virgo Cluster; Globular cluster; Galaxy; Galaxy cluster; Population; Halo; Cluster (spacecraft); Stars","score_opus":0.035967923670708266,"score_gpt":0.27046463517895897,"score_spread":0.2344967115082507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788675381","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96116513,0.0004481119,0.00033365496,0.00012107627,0.000010076415,0.000054640375,0.031997517,0.00008655333,0.005783149],"genre_scores_gemma":[0.9424887,0.00023384814,0.0008959187,0.0001170483,0.000013354052,0.000036587226,0.05227912,0.000017840272,0.003917587],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991035,0.000011361862,0.0000041617614,0.00002061421,0.000027254651,0.000026221742],"domain_scores_gemma":[0.9997924,0.000015353966,0.00004826433,0.00002358883,0.00003992909,0.00008053262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016829501,0.000085913845,0.000105198196,0.0013722654,0.00018755226,0.0002681705,0.00018194699,0.0001290519,0.0026366476],"category_scores_gemma":[0.00029901764,0.000052178875,0.00011291888,0.0010220201,0.00008075859,0.000094818824,0.00038480348,0.0001018861,0.0007943053],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006176106,0.000023527386,0.97615844,0.00003714929,0.000048652022,0.00008901365,0.00015134974,0.00012764889,0.0030070446,0.00027233968,0.0071997033,0.0128232725],"study_design_scores_gemma":[0.000001808357,0.0000060164048,0.9967526,0.000004376243,0.0000055788187,0.00003393311,0.000052332263,0.00013380243,0.00014802671,0.000025769763,0.0028350337,8.5346477e-7],"about_ca_topic_score_codex":0.034316435,"about_ca_topic_score_gemma":0.051854026,"teacher_disagreement_score":0.034316435,"about_ca_system_score_codex":0.00033465197,"about_ca_system_score_gemma":0.00023807614,"threshold_uncertainty_score":0.06823337},"labels":[],"label_agreement":null},{"id":"W2788809511","doi":"10.3847/1538-4357/aaaf1a","title":"The Cocoon Shocks of Cygnus A: Pressures and Their Implications for the Jets and Lobes","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Mach number; Jet (fluid); Kinetic energy; Shock (circulatory); Flux (metallurgy); Shock wave; Momentum (technical analysis); Synchrotron; Mechanics; Nuclear physics; Classical mechanics","score_opus":0.0113341480487542,"score_gpt":0.245794151258408,"score_spread":0.2344600032096538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2788809511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981572,0.00015284018,0.00041719418,0.000050232527,0.000004101429,0.0000058416504,0.00014426399,0.00003575586,0.001032638],"genre_scores_gemma":[0.99974066,0.00003690108,0.000100892,0.0000071079494,0.0000053851127,0.0000023798184,0.00005208146,0.000004186849,0.000050418465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994016,0.000009753953,0.000003546329,0.000015653077,0.000014733286,0.00001609935],"domain_scores_gemma":[0.99948186,0.00021971628,0.00017004512,0.000026908072,0.000034776163,0.000066770335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019507672,0.00024338478,0.00015996944,0.0007877883,0.00029914622,0.00080373354,0.00023329062,0.00022925674,0.0007197226],"category_scores_gemma":[0.0011376678,0.00014645838,0.00019410133,0.00058071624,0.00028234159,0.00029852343,0.00046454548,0.00026375282,0.00010175638],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000893134,0.000094849565,0.8744372,0.00007986189,0.00010977148,0.0021729253,0.00048065544,0.014348215,0.08729187,0.0021874276,0.0006930365,0.017211141],"study_design_scores_gemma":[0.000014539299,0.00005035904,0.97873497,0.0000068882,0.000015234367,0.00023482344,0.0001077876,0.015891358,0.0040908633,0.0005558334,0.00028665204,0.000010696628],"about_ca_topic_score_codex":0.0060167597,"about_ca_topic_score_gemma":0.0031381901,"teacher_disagreement_score":0.0060167597,"about_ca_system_score_codex":0.0007908119,"about_ca_system_score_gemma":0.00017003414,"threshold_uncertainty_score":0.011963487},"labels":[],"label_agreement":null},{"id":"W2789001403","doi":"10.3847/1538-4357/aaafc7","title":"The Envelope Kinematics and a Possible Disk around the Class 0 Protostar within BHR7","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Smithsonian Astrophysical Observatory; Smithsonian Institution; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; European Space Agency; Academia Sinica","keywords":"Physics; Protostar; Astrophysics; Submillimeter Array; Millimeter; Angular momentum; Molecular cloud; Bipolar outflow; Astronomy; Star formation; Stars","score_opus":0.011573195216433137,"score_gpt":0.24801775996924028,"score_spread":0.23644456475280715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2789001403","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988967,0.000046986996,0.0002271485,0.000009579794,0.0000011517102,0.0000019692814,0.000023277758,0.000006283865,0.000786868],"genre_scores_gemma":[0.9996172,0.000012595094,0.00018913616,0.000004058662,0.0000023102325,7.2825287e-7,0.00005643147,0.0000022531635,0.00011520058],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994993,0.0000050518956,0.0000022739016,0.00001085507,0.000015160711,0.000016754911],"domain_scores_gemma":[0.99982697,0.000018532437,0.00005946758,0.000016438446,0.000025737421,0.000052847143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000072487535,0.00011599056,0.00013170284,0.00040110768,0.00032857832,0.00047109489,0.00026320294,0.00020457711,0.0010054332],"category_scores_gemma":[0.00020236972,0.00010545672,0.00009820479,0.0001806634,0.000343273,0.00022707974,0.00038474333,0.000103046885,0.0004081108],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022197182,0.000087901,0.7055304,0.000031487674,0.000037282865,0.001637652,0.0005507053,0.00083898247,0.2777659,0.0017079224,0.00019427089,0.011395433],"study_design_scores_gemma":[0.000009819021,0.00017230363,0.9802617,0.000013837586,0.000019117353,0.0011931078,0.00074263255,0.0047107576,0.010633243,0.0008691426,0.00136382,0.000010562338],"about_ca_topic_score_codex":0.001578985,"about_ca_topic_score_gemma":0.001588846,"teacher_disagreement_score":0.001578985,"about_ca_system_score_codex":0.00021532663,"about_ca_system_score_gemma":0.00007327985,"threshold_uncertainty_score":0.0033635497},"labels":[],"label_agreement":null},{"id":"W2789788694","doi":"10.3847/1538-4357/aab767","title":"Habitability from Tidally Induced Tectonics","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"High-pressure geophysics and materials","field":"Earth and Planetary Sciences","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Toronto","funders":"","keywords":"Habitability; Terrestrial planet; Outgassing; Planet; Planetary habitability; Circumstellar habitable zone; Tectonics; Defrosting","score_opus":0.012324072058861251,"score_gpt":0.21305135177623213,"score_spread":0.2007272797173709,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2789788694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96202946,0.00021543512,0.015822664,0.0005794651,0.000041282517,0.000013892389,0.00037304056,0.00023648287,0.020688294],"genre_scores_gemma":[0.9989059,0.000031777854,0.00026688288,0.000024360976,0.000008602958,0.0000033714869,0.00006731518,0.000014265763,0.00067741633],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999262,0.000010380212,0.000005158901,0.000025056028,0.000012439919,0.000020790867],"domain_scores_gemma":[0.9994803,0.0000692774,0.00014287158,0.00015864744,0.00004429654,0.00010456865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017324142,0.000216988,0.0002744701,0.0003283882,0.0004995362,0.0010103326,0.00036894312,0.0004408993,0.0057090134],"category_scores_gemma":[0.0011791313,0.00016153594,0.0004353344,0.00019079079,0.0010869426,0.0011676074,0.0011812577,0.0005053624,0.0003876603],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005860787,0.00009900932,0.2407602,0.00026849675,0.00034949163,0.0016478285,0.0015687017,0.15097591,0.08233765,0.46315342,0.005482868,0.0527704],"study_design_scores_gemma":[0.00005842816,0.00019066865,0.24192125,0.000054243323,0.000087827655,0.0011612681,0.00053844537,0.29091683,0.007192912,0.4457988,0.011954993,0.00012420365],"about_ca_topic_score_codex":0.0026361686,"about_ca_topic_score_gemma":0.0015710802,"teacher_disagreement_score":0.0057090134,"about_ca_system_score_codex":0.0005888888,"about_ca_system_score_gemma":0.00023789731,"threshold_uncertainty_score":0.01909858},"labels":[],"label_agreement":null},{"id":"W2789955199","doi":"10.3847/1538-4357/aaaa6d","title":"A Color-locus Method for Mapping R<sub>V</sub> Using Ensembles of Stars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Harvard University; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Stars; Galactic plane; Observable; Pixel; Monte Carlo method; Spectral line; Simple (philosophy)","score_opus":0.026385112523846798,"score_gpt":0.2743602206052632,"score_spread":0.24797510808141643,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2789955199","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04467901,0.000049124203,0.9527465,0.00003091027,0.000013594585,0.000026231102,0.00019734022,0.001480795,0.00077636883],"genre_scores_gemma":[0.41947868,0.000041519143,0.57765913,0.000052438383,0.000024184343,0.00008398303,0.0007383627,0.00035085742,0.0015708205],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995041,0.00012937897,0.000023611958,0.00017443663,0.00013212237,0.00003640979],"domain_scores_gemma":[0.9984257,0.0003975284,0.00017986387,0.0005529846,0.0003541338,0.00008984514],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013943095,0.00027765904,0.00034801767,0.0012470055,0.00047109468,0.000719328,0.00096437475,0.00039426787,0.00208521],"category_scores_gemma":[0.0043459977,0.0002560621,0.0004353344,0.0006759952,0.0003497554,0.00054357614,0.0009383444,0.00044814235,0.00086406094],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002986901,0.00018224516,0.08013276,0.00007417492,0.00035489816,0.0001507496,0.00039988596,0.116575934,0.0628179,0.024149647,0.0031436004,0.7117195],"study_design_scores_gemma":[0.000029928604,0.00007644651,0.02696834,0.000013912057,0.000046965375,0.00023950342,0.00006863242,0.9282657,0.02405267,0.015933309,0.0042401673,0.00006442785],"about_ca_topic_score_codex":0.0028887664,"about_ca_topic_score_gemma":0.0036167658,"teacher_disagreement_score":0.0028887664,"about_ca_system_score_codex":0.00029192006,"about_ca_system_score_gemma":0.0005030567,"threshold_uncertainty_score":0.007373929},"labels":[],"label_agreement":null},{"id":"W2789993401","doi":"10.3847/1538-4357/aab713","title":"On the Spectral Evolution of Helium-atmosphere White Dwarfs Showing Traces of Hydrogen","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"White dwarf; Brown dwarf; Hydrogen; Stellar classification; Stars; Population; Spectral line; Accretion (finance); Convection","score_opus":0.010054379940390929,"score_gpt":0.2134779100361275,"score_spread":0.20342353009573658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2789993401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997464,0.000019609044,0.00006786565,0.0000014688968,3.3871538e-7,6.3462215e-7,0.000047170925,0.0000030934045,0.00011341245],"genre_scores_gemma":[0.9997708,0.000007913571,0.00005544612,0.0000014013793,5.709079e-7,4.780004e-7,0.00010498951,0.0000012344294,0.000057107398],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995005,0.0000070701817,0.00000426737,0.000016544765,0.000010749786,0.000011271139],"domain_scores_gemma":[0.9996574,0.00006329109,0.00008325489,0.000026784212,0.000050639388,0.000118562195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019889315,0.000172551,0.0001721592,0.00074001675,0.0002873739,0.00030605978,0.00014095055,0.00014708802,0.00044527615],"category_scores_gemma":[0.00040013093,0.000069399895,0.00012950457,0.00038860235,0.00020496272,0.00014299265,0.00022539485,0.00008123337,0.00018719619],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016877032,0.000026609561,0.97236246,0.00000655813,0.000023508466,0.00016060006,0.00016664667,0.00030416923,0.02465525,0.000090422,0.000032744214,0.0020021866],"study_design_scores_gemma":[0.0000018881625,0.00008069932,0.99572766,0.0000011025313,0.0000089405985,0.00031249964,0.00013773143,0.0009575265,0.0025575885,0.000062505176,0.00014978633,0.0000020957139],"about_ca_topic_score_codex":0.0016286093,"about_ca_topic_score_gemma":0.0022094934,"teacher_disagreement_score":0.0016286093,"about_ca_system_score_codex":0.00015145267,"about_ca_system_score_gemma":0.00006421181,"threshold_uncertainty_score":0.0032383204},"labels":[],"label_agreement":null},{"id":"W2790248196","doi":"10.3847/1538-4357/aab3c9","title":"X-Ray Scaling Relations of Early-type Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; University of Waterloo; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Luminosity; Scaling; Galaxy; Supernova; Gravitational potential; Mass fraction; Thermodynamics; Geometry","score_opus":0.00979462506170166,"score_gpt":0.22548861866078104,"score_spread":0.21569399359907937,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790248196","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993674,0.00005236422,0.0001403669,0.000005627316,4.511891e-7,0.0000020117488,0.00012393847,0.000009701809,0.00029811673],"genre_scores_gemma":[0.999539,0.00002370805,0.00013960729,0.0000023754253,0.0000014226117,0.0000022946053,0.00020126124,0.000002203382,0.000088042245],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987626,0.000024216668,0.000012665795,0.00003317225,0.000025619915,0.000028103887],"domain_scores_gemma":[0.9975746,0.0007537477,0.0007709125,0.00023988124,0.00034823053,0.00031254414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005593309,0.0002321293,0.00016652839,0.0017790571,0.00020844222,0.00061779475,0.0002769267,0.00017738891,0.0009272091],"category_scores_gemma":[0.0022221727,0.00012558002,0.00019914193,0.0007044204,0.0002922648,0.0002568739,0.00032986957,0.00022766767,0.00023577876],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056157623,0.00001834177,0.992547,0.0000073225215,0.00002275361,0.00005088905,0.00015784679,0.000875034,0.00282041,0.0002334754,0.00006396146,0.0031467807],"study_design_scores_gemma":[0.0000018915256,0.000015432448,0.99848914,0.0000013265513,0.0000032858395,0.000049423692,0.000037122274,0.0008960894,0.0003031527,0.00011758894,0.000083674684,0.000001881526],"about_ca_topic_score_codex":0.003332579,"about_ca_topic_score_gemma":0.0024019661,"teacher_disagreement_score":0.003332579,"about_ca_system_score_codex":0.00040736783,"about_ca_system_score_gemma":0.00007305331,"threshold_uncertainty_score":0.0066263676},"labels":[],"label_agreement":null},{"id":"W2790274533","doi":"10.3847/1538-4357/aaacd7","title":"Resolved Millimeter Observations of the HR 8799 Debris Disk","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Planetesimal; Debris disk; Planet; Debris; Millimeter; Planetary system; Population; Giant planet","score_opus":0.023838307780008502,"score_gpt":0.24721352965600013,"score_spread":0.22337522187599163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790274533","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956726,0.00020408741,0.00074982754,0.000036730988,0.000008442892,0.000006056346,0.00076902774,0.00013255245,0.002420795],"genre_scores_gemma":[0.99736196,0.000057117282,0.0011896207,0.00002452597,0.000015267406,0.000006305847,0.0010017497,0.0000080353275,0.0003354948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.000007639867,0.00000429371,0.000017764953,0.000034114677,0.000019128314],"domain_scores_gemma":[0.9997782,0.000030486795,0.00007436652,0.000042128268,0.00003672153,0.000038138707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015174162,0.00013165701,0.00017759045,0.0006155089,0.00018918885,0.00031266588,0.0002388123,0.00018222998,0.00062227296],"category_scores_gemma":[0.0002809951,0.00013057778,0.00012249924,0.00039855772,0.00007164712,0.0001278256,0.00028628143,0.00022290359,0.00027333206],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072591804,0.000258022,0.6135579,0.00012500127,0.0002595545,0.0010476639,0.0005151152,0.0033223643,0.30337426,0.0012277206,0.006456123,0.0691304],"study_design_scores_gemma":[0.000023956207,0.00005080581,0.9886165,0.000010981399,0.000029902594,0.00019707595,0.000056788405,0.0021220054,0.005669355,0.00010174549,0.0031145448,0.0000062134914],"about_ca_topic_score_codex":0.0014044818,"about_ca_topic_score_gemma":0.0030758479,"teacher_disagreement_score":0.0014044818,"about_ca_system_score_codex":0.00019533858,"about_ca_system_score_gemma":0.00006424617,"threshold_uncertainty_score":0.0027925968},"labels":[],"label_agreement":null},{"id":"W2790288751","doi":"10.3847/1538-4357/aab892","title":"Color Dispersion as an Indicator of Stellar Population Complexity: Insights from the Pixel Color–Magnitude Diagrams of 32 Bright Galaxies in Abell 1139 and Abell 2589","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Elliptical galaxy; Lenticular galaxy; Galaxy; Surface brightness fluctuation; Astronomy; Irregular galaxy; Bulge; Population","score_opus":0.010491739936323878,"score_gpt":0.22560600515991863,"score_spread":0.21511426522359475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790288751","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904984,0.000035393434,0.0002384085,0.000008847768,7.6939494e-7,0.0000016726927,0.0003019209,0.00002075237,0.00034240072],"genre_scores_gemma":[0.99908924,0.000011777239,0.00037059182,0.0000033005126,0.000001914936,0.0000015999569,0.00045599072,0.0000046710684,0.000061008705],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.00001846292,0.000011611483,0.000031308577,0.00003396894,0.000026867849],"domain_scores_gemma":[0.9989637,0.00021359096,0.00036065106,0.00007031563,0.00014962576,0.00024227229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026507053,0.000120913275,0.00024964538,0.0027169164,0.00025019652,0.000706644,0.00014987055,0.0002190311,0.0011499642],"category_scores_gemma":[0.0009239057,0.000115360825,0.00016928528,0.0011404364,0.00021747223,0.00027582346,0.00033802746,0.00016332045,0.0002775389],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018185524,0.00003807366,0.9711628,0.000015180025,0.00003736931,0.00009925911,0.00016475318,0.0004882076,0.022127915,0.00015215571,0.00015088354,0.0053816014],"study_design_scores_gemma":[0.0000010619094,0.000011247957,0.9987256,8.547383e-7,0.00000397702,0.000040160234,0.00005120213,0.00063377136,0.00042056633,0.00002650372,0.00008306726,0.000001935522],"about_ca_topic_score_codex":0.0057675703,"about_ca_topic_score_gemma":0.007955011,"teacher_disagreement_score":0.0057675703,"about_ca_system_score_codex":0.00033680443,"about_ca_system_score_gemma":0.00011367373,"threshold_uncertainty_score":0.011468053},"labels":[],"label_agreement":null},{"id":"W2790557288","doi":"10.3847/1538-4357/aab61d","title":"The Green Bank Northern Celestial Cap Pulsar Survey. II. The Discovery and Timing of 10 Pulsars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; European Commission; National Science Foundation","keywords":"Pulsar; Neutron star; Binary pulsar; Millisecond pulsar; Green Bank Telescope; X-ray pulsar; Pulsar planet; Binary number","score_opus":0.017181688927607724,"score_gpt":0.30414757425923117,"score_spread":0.2869658853316234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790557288","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9537688,0.0018568814,0.00072049076,0.0006085664,0.000104396546,0.000077556964,0.020928591,0.00018911868,0.021745535],"genre_scores_gemma":[0.965501,0.0013185982,0.002718718,0.00033951775,0.0001150122,0.00008286894,0.021009212,0.0000680099,0.008847193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996227,0.000051079875,0.000022817248,0.000076529774,0.00012191647,0.00010494963],"domain_scores_gemma":[0.9987336,0.00011731493,0.00029780777,0.00012057667,0.00043252952,0.00029818263],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054770004,0.00026448764,0.00028572,0.003286127,0.00077502313,0.0010122018,0.00037848577,0.00030881728,0.0029807335],"category_scores_gemma":[0.001108729,0.00023503092,0.00013962224,0.003260701,0.00034569108,0.00035310216,0.000665284,0.00024817,0.0014593474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037783387,0.00003401906,0.9445741,0.00005956853,0.000052625925,0.0005524157,0.00032485154,0.00041770283,0.002963696,0.00033732972,0.015315932,0.034989875],"study_design_scores_gemma":[0.000023448334,0.00003166137,0.9803743,0.000027909287,0.0000134079155,0.00024327888,0.00027082113,0.00073847454,0.0006424047,0.000059900263,0.017563727,0.000010649815],"about_ca_topic_score_codex":0.21393026,"about_ca_topic_score_gemma":0.3501956,"teacher_disagreement_score":0.21393026,"about_ca_system_score_codex":0.0017968125,"about_ca_system_score_gemma":0.0012572082,"threshold_uncertainty_score":0.4253701},"labels":[],"label_agreement":null},{"id":"W2790645022","doi":"10.3847/1538-4357/aab890","title":"ALMA Survey of Lupus Protoplanetary Disks. II. Gas Disk Radii","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":361,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Millimeter; Planet; Dimensionless quantity; Submillimeter Array; Systemic lupus erythematosus; Protoplanetary disk; Accretion (finance); Accretion disc","score_opus":0.015115715598738,"score_gpt":0.24709963426285264,"score_spread":0.23198391866411464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790645022","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99579877,0.000457196,0.00026814864,0.00003809385,0.000003817049,0.000009691728,0.0017036843,0.00006848418,0.0016520473],"genre_scores_gemma":[0.99655944,0.00012861441,0.0006854917,0.000022999711,0.000017526114,0.00001302624,0.0019778106,0.000007943622,0.00058699254],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998266,0.000022290767,0.000010824416,0.000054848177,0.00005116924,0.000034322555],"domain_scores_gemma":[0.9994386,0.000058387363,0.00020575062,0.000051160747,0.00011269709,0.00013338425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024006401,0.00018723082,0.00019273054,0.001677035,0.00028644278,0.00039555217,0.0003183505,0.0001584959,0.0011397908],"category_scores_gemma":[0.0004967779,0.00010131005,0.0001633058,0.0005783006,0.00011408876,0.0002737637,0.00036296775,0.00014920096,0.00049351493],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015289673,0.00003459289,0.96839595,0.00004709086,0.0000511641,0.00012241365,0.00025148498,0.0002077849,0.013372021,0.00012038911,0.0008331844,0.016411163],"study_design_scores_gemma":[0.000006080878,0.000028442246,0.99616724,0.0000044527155,0.000009740987,0.0001531674,0.00005870025,0.00033639593,0.00077013986,0.00002057309,0.002442775,0.0000024203982],"about_ca_topic_score_codex":0.0035838766,"about_ca_topic_score_gemma":0.0051665865,"teacher_disagreement_score":0.0035838766,"about_ca_system_score_codex":0.00040372144,"about_ca_system_score_gemma":0.00011827302,"threshold_uncertainty_score":0.0071260333},"labels":[],"label_agreement":null},{"id":"W2790790236","doi":"10.1088/0004-637x/771/1/72","title":"EXTINCTION AND POLYCYCLIC AROMATIC HYDROCARBON INTENSITY VARIATIONS ACROSS THE H II REGION IRAS 12063–6259","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Extinction (optical mineralogy); Intensity (physics); Absorption (acoustics); Silicate; Measure (data warehouse); Magnitude (astronomy); Polycyclic aromatic hydrocarbon; Optical depth","score_opus":0.010799530048907897,"score_gpt":0.23074604393874049,"score_spread":0.21994651388983258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790790236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972516,0.00015206297,0.00026152903,0.000017893139,0.0000042380975,0.0000040151263,0.000175809,0.000038221206,0.00209461],"genre_scores_gemma":[0.999015,0.000052805633,0.00019930633,0.000020809313,0.0000068863615,0.0000042856736,0.00047448062,0.000010445385,0.00021595374],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998628,0.00000764928,0.0000090623125,0.000055435623,0.00004103917,0.000023989607],"domain_scores_gemma":[0.9996903,0.000026818934,0.00012968437,0.000032563883,0.00005369906,0.00006691585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001373604,0.00021874705,0.00019037248,0.00079633034,0.00020250175,0.00044933514,0.00024405963,0.00025343627,0.0006471543],"category_scores_gemma":[0.00039254368,0.00015294761,0.00019868936,0.0006042361,0.00024166626,0.00024396842,0.0003508302,0.00024039771,0.00041695175],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002977964,0.00020898222,0.7571948,0.000046817655,0.00017551892,0.00028046695,0.00051057857,0.0017200625,0.21239671,0.00037794223,0.00069870456,0.026091643],"study_design_scores_gemma":[0.000004499475,0.000018353176,0.99790263,0.0000021896383,0.000011411928,0.000034791658,0.000039735933,0.00045067654,0.0012895676,0.000039099148,0.00020477542,0.0000023508264],"about_ca_topic_score_codex":0.004458339,"about_ca_topic_score_gemma":0.004617142,"teacher_disagreement_score":0.004458339,"about_ca_system_score_codex":0.00021952932,"about_ca_system_score_gemma":0.000059468555,"threshold_uncertainty_score":0.00886476},"labels":[],"label_agreement":null},{"id":"W2790986222","doi":"10.3847/1538-4357/aab371","title":"A Strong Limit on the Very-high-energy Emission from GRB 150323A","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Gamma-ray burst; Astrophysics; Limit (mathematics); Astronomy","score_opus":0.013492177041045599,"score_gpt":0.22237146117767334,"score_spread":0.20887928413662774,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2790986222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9829144,0.0017476005,0.0024535973,0.00040379228,0.000049380214,0.000020191366,0.0009775698,0.0002485316,0.011185021],"genre_scores_gemma":[0.99808854,0.0000722929,0.0005488839,0.00018880551,0.000017410332,0.000013786399,0.0007467645,0.000019193527,0.0003042362],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99963915,0.000033307333,0.000028400078,0.000117682284,0.00009396508,0.00008746138],"domain_scores_gemma":[0.9988525,0.00026108694,0.0003615808,0.00015367036,0.00012308317,0.0002480543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000672572,0.0003168514,0.00043967317,0.0006382625,0.00039887527,0.0011414341,0.00047774636,0.0011173998,0.0036811468],"category_scores_gemma":[0.0019746574,0.00029536374,0.00028385577,0.00042458743,0.00050585327,0.0005822742,0.0009330462,0.0008930269,0.0012151322],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014420245,0.0001937966,0.32671276,0.0003013972,0.00012954616,0.0017418339,0.0005223733,0.00092408556,0.6334426,0.004978231,0.0038794028,0.025731893],"study_design_scores_gemma":[0.00005926502,0.0003398729,0.9418322,0.00019610286,0.000041704636,0.0059942296,0.00025349297,0.002357526,0.034646686,0.004302024,0.009916794,0.000060067272],"about_ca_topic_score_codex":0.0013328564,"about_ca_topic_score_gemma":0.0017248163,"teacher_disagreement_score":0.0036811468,"about_ca_system_score_codex":0.00044379555,"about_ca_system_score_gemma":0.0002249215,"threshold_uncertainty_score":0.012314677},"labels":[],"label_agreement":null},{"id":"W2791204014","doi":"10.3847/1538-4357/aaaab0","title":"The LABOCA/ACT Survey of Clusters at All Redshifts: Multiwavelength Analysis of Background Submillimeter Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Redshift; Galaxy; Bolometer; Telescope; Cosmology; Millimeter; Galaxy cluster; Sky; Radio telescope; South Pole Telescope","score_opus":0.019248534694532915,"score_gpt":0.250686015212868,"score_spread":0.23143748051833507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2791204014","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99436533,0.00014634688,0.00070001103,0.00004313432,0.0000036301633,0.000016544042,0.002764298,0.00012589003,0.0018348774],"genre_scores_gemma":[0.9918576,0.0000702444,0.0020887435,0.000035403697,0.000018447103,0.000026463393,0.005202674,0.00004902713,0.00065138104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954104,0.00006283959,0.00001946095,0.00012521398,0.00015712857,0.00009439207],"domain_scores_gemma":[0.9985709,0.00014700831,0.0003310594,0.00030087036,0.00034716586,0.00030305318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046826043,0.00023611735,0.00033705562,0.0034604657,0.0004337171,0.00093187694,0.0003754896,0.0001531642,0.0013975538],"category_scores_gemma":[0.0008738504,0.00015402169,0.0003915161,0.0017753314,0.00019824752,0.00026089765,0.0008746139,0.0002686567,0.0005056823],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016671629,0.000040784656,0.9716699,0.000023302331,0.000115674215,0.00009899737,0.00023992154,0.00085530995,0.011928166,0.00023592543,0.0017951308,0.012830152],"study_design_scores_gemma":[0.000002948471,0.0000094205325,0.9974432,0.0000019988765,0.000014720747,0.000034713346,0.00007626059,0.0009898423,0.00051629415,0.000023155299,0.00088347786,0.0000039832325],"about_ca_topic_score_codex":0.03222656,"about_ca_topic_score_gemma":0.054326333,"teacher_disagreement_score":0.03222656,"about_ca_system_score_codex":0.00039418647,"about_ca_system_score_gemma":0.00042365186,"threshold_uncertainty_score":0.06407797},"labels":[],"label_agreement":null},{"id":"W2791445767","doi":"10.3847/1538-4357/aab3d4","title":"Aspherical Supernovae: Effects on Early Light Curves","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Ejecta; Light curve; Adiabatic process; Mixing (physics); Breakout; Luminosity; Shock (circulatory); Polytropic process; Photon","score_opus":0.007974678985966986,"score_gpt":0.2288346945823829,"score_spread":0.2208600155964159,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2791445767","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977518,0.000059233556,0.0006522696,0.00004850615,0.0000041743415,0.0000044543276,0.00016586753,0.00004355297,0.0012703245],"genre_scores_gemma":[0.99953365,0.00003367982,0.00013446846,0.0000090173,0.0000016611289,0.0000026825614,0.00007905543,0.000016461481,0.00018935966],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999926,0.000025788127,0.0000040182613,0.00001282006,0.000011777628,0.00001955665],"domain_scores_gemma":[0.99914813,0.00044269764,0.00011396229,0.000079931524,0.00005796251,0.000157281],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002598245,0.00036810225,0.0002750805,0.0002804737,0.00026557822,0.00057716295,0.00036676784,0.00029723495,0.0018409567],"category_scores_gemma":[0.001528579,0.00012464302,0.0003230599,0.0002390998,0.00037041184,0.00032194197,0.0005301415,0.00045206604,0.00011178743],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007165343,0.0002728022,0.082104675,0.000097881995,0.00018733332,0.0005798617,0.00023373964,0.85702634,0.04542231,0.0054099746,0.00065947685,0.0072890865],"study_design_scores_gemma":[0.00014120218,0.0004269503,0.08853736,0.000019318582,0.000080060774,0.00013017363,0.00015684575,0.8931777,0.013256195,0.0031212012,0.0009092474,0.000043761673],"about_ca_topic_score_codex":0.004393842,"about_ca_topic_score_gemma":0.0023156141,"teacher_disagreement_score":0.004393842,"about_ca_system_score_codex":0.00042325043,"about_ca_system_score_gemma":0.00018681266,"threshold_uncertainty_score":0.008736551},"labels":[],"label_agreement":null},{"id":"W2791464542","doi":"10.3847/1538-4357/aaa757","title":"Polycyclic Aromatic Hydrocarbons with Straight Edges and the 7.6/6.2 and 8.6/6.2 Intensity Ratios in Reflection Nebulae","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Aeronautics and Space Administration","keywords":"Reflection nebula; Carbon fibers; Absorption (acoustics); Photodissociation; Reflection (computer programming); Infrared; Physics; Intensity (physics); Radiant intensity; Irradiation; Photochemistry; Astrophysics; Analytical Chemistry (journal); Materials science; Radiation; Chemistry; Environmental chemistry; Optics; Planetary nebula","score_opus":0.009735348833026278,"score_gpt":0.23250078527636317,"score_spread":0.2227654364433369,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2791464542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950459,0.00009817363,0.00351795,0.000023326733,0.0000025316644,0.0000045330175,0.00011459045,0.00004628107,0.0011466468],"genre_scores_gemma":[0.99897975,0.000023419178,0.0007928823,0.0000067583023,8.311074e-7,0.000002424821,0.00008664464,0.000006438303,0.00010076177],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999474,0.000009558279,0.0000016944911,0.000010210225,0.000014244213,0.000017003991],"domain_scores_gemma":[0.9998754,0.00004283746,0.000033553133,0.000011821515,0.000020029873,0.000016351181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019419371,0.00022391409,0.00010801391,0.0003423894,0.00017629088,0.00018852366,0.0002991682,0.00021402627,0.0014462142],"category_scores_gemma":[0.0003009229,0.00013224762,0.00029872442,0.00025076684,0.00023891771,0.00021289548,0.00016646982,0.00026611963,0.00010880682],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005609857,0.00034025067,0.26839802,0.00020646576,0.00021933796,0.0006646478,0.00021474244,0.11671748,0.5746809,0.019391257,0.00059415225,0.01801165],"study_design_scores_gemma":[0.00008726046,0.00025414603,0.3474082,0.000023668792,0.00009030204,0.0005390402,0.00020018854,0.46678978,0.17312342,0.010035759,0.0013827574,0.0000654621],"about_ca_topic_score_codex":0.0019214299,"about_ca_topic_score_gemma":0.0019837967,"teacher_disagreement_score":0.0019214299,"about_ca_system_score_codex":0.0002770519,"about_ca_system_score_gemma":0.000115856565,"threshold_uncertainty_score":0.0048380494},"labels":[],"label_agreement":null},{"id":"W2791788057","doi":"10.3847/1538-4357/aab88a","title":"Stellar Population Properties of Ultracompact Dwarfs in M87: A Mass–Metallicity Correlation Connecting Low-metallicity Globular Clusters and Compact Ellipticals","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Virgo Cluster; Stellar population; Galaxy; Elliptical galaxy; Star cluster; Population; Stellar density","score_opus":0.0120170039051049,"score_gpt":0.22289855152298751,"score_spread":0.2108815476178826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2791788057","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997464,0.000034863584,0.00006627559,0.0000022764264,2.103625e-7,6.763795e-7,0.000037842543,0.00000243106,0.00010891614],"genre_scores_gemma":[0.99972326,0.000016626542,0.000054636825,0.0000020537511,0.0000010510341,8.072604e-7,0.00016511563,0.0000011475738,0.00003526589],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998685,0.00001856682,0.00001285902,0.000036338617,0.000032071744,0.00003168229],"domain_scores_gemma":[0.9991129,0.0002048764,0.00026547385,0.00012374017,0.00014910776,0.00014388622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003125276,0.00019147366,0.00028461262,0.0016419017,0.00023803234,0.00057774637,0.00028392344,0.0001737942,0.0005480643],"category_scores_gemma":[0.0012852565,0.00009146547,0.00016187732,0.0007544542,0.0003392046,0.00018836951,0.0005963427,0.000108516375,0.0003105803],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000020343896,0.0000062491167,0.99758923,0.0000028006878,0.000015381165,0.000029994875,0.00009601006,0.00023213538,0.00083098415,0.00004714992,0.000026400374,0.0011033466],"study_design_scores_gemma":[9.236019e-7,0.000009821434,0.9986216,0.0000015616961,0.0000072290923,0.00005743116,0.000095807685,0.0007887693,0.00027535978,0.00004965136,0.00009067292,0.0000010529202],"about_ca_topic_score_codex":0.0025651068,"about_ca_topic_score_gemma":0.0028797868,"teacher_disagreement_score":0.0025651068,"about_ca_system_score_codex":0.00025953606,"about_ca_system_score_gemma":0.00008955585,"threshold_uncertainty_score":0.00510031},"labels":[],"label_agreement":null},{"id":"W2792118602","doi":"10.3847/1538-4357/aab432","title":"Photospheric Observations of Surface and Body Modes in Solar Magnetic Pores","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Queen's University; Queen's University Belfast; Leverhulme Trust; Department of Science and Technology, Ministry of Science and Technology, India; Invest Northern Ireland; National Science Foundation","keywords":"Physics; Helioseismology; Surface (topology); Astronomy; Astrophysics; Solar physics; Astrobiology; Solar atmosphere; Magnetic field; Geometry","score_opus":0.009973394765902666,"score_gpt":0.2244058774122543,"score_spread":0.21443248264635162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2792118602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99664634,0.000091901464,0.0005953508,0.000029606532,0.000004687204,0.0000041154235,0.00020078523,0.00004574119,0.0023814964],"genre_scores_gemma":[0.99936146,0.000026974147,0.00028966303,0.0000069972116,0.000004004809,0.0000024656165,0.000119805954,0.0000059118024,0.00018271658],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999447,0.000005095465,0.0000018027345,0.000013973303,0.000021440335,0.000012977919],"domain_scores_gemma":[0.99969745,0.00008598923,0.000060309674,0.000030442992,0.00005849239,0.00006735521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013293794,0.00010105416,0.0001397589,0.00086265465,0.00028186876,0.00033590867,0.00014420747,0.0002441704,0.0013509748],"category_scores_gemma":[0.00035629235,0.00011703222,0.00009987982,0.00040556354,0.00033834454,0.00034766019,0.000449828,0.00027882814,0.0002173545],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045770535,0.0000812972,0.43300432,0.000091587084,0.00006534475,0.00035749603,0.0013659326,0.0006210857,0.53215635,0.0007800825,0.0012845284,0.02973434],"study_design_scores_gemma":[0.000011778262,0.000075366464,0.98552483,0.000010284427,0.000011324257,0.00021898458,0.0005308403,0.0012052748,0.010180068,0.00026810038,0.0019538973,0.000009217563],"about_ca_topic_score_codex":0.0007481082,"about_ca_topic_score_gemma":0.0015786098,"teacher_disagreement_score":0.0013509748,"about_ca_system_score_codex":0.000095797724,"about_ca_system_score_gemma":0.0000400344,"threshold_uncertainty_score":0.0045194626},"labels":[],"label_agreement":null},{"id":"W2793681743","doi":"10.3847/1538-4357/aab711","title":"Magnetic Fields Recorded by Chondrules Formed in Nebular Shocks","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Chondrule; Physics; Magnetic field; Astrophysics; Astrobiology; Geophysics; Meteorite; Chondrite","score_opus":0.0055870627089191416,"score_gpt":0.20671896423196248,"score_spread":0.20113190152304333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2793681743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994388,0.000020466792,0.00015482487,0.000004978214,8.9014145e-7,0.000001874834,0.0000733509,0.000016574832,0.0002883286],"genre_scores_gemma":[0.9995509,0.000011711329,0.00014732881,0.0000021409858,0.0000010350001,0.0000011962221,0.00016304625,0.0000038691196,0.00011865714],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999535,0.0000037854156,0.0000030437272,0.000013823175,0.000011044637,0.000014668807],"domain_scores_gemma":[0.99983513,0.000036827678,0.000040213938,0.000016435288,0.000028582386,0.00004278866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011732196,0.00015664069,0.00021336754,0.00032201258,0.00023104162,0.0004189644,0.00025057278,0.00026720142,0.00074774143],"category_scores_gemma":[0.000515359,0.00015638028,0.00027938775,0.00022251562,0.0002387021,0.00019164408,0.00039029046,0.00023255442,0.00013800278],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076738826,0.00007694816,0.55305105,0.00006874518,0.00015871375,0.0012775499,0.0005093713,0.08992416,0.34437114,0.0011626313,0.0003051591,0.008327105],"study_design_scores_gemma":[0.0000611932,0.0001801835,0.8395551,0.000010606841,0.000031325922,0.00031605733,0.00025530916,0.12785698,0.030612376,0.00032181112,0.0007753304,0.000023656175],"about_ca_topic_score_codex":0.0050972495,"about_ca_topic_score_gemma":0.0027128805,"teacher_disagreement_score":0.0050972495,"about_ca_system_score_codex":0.0005981666,"about_ca_system_score_gemma":0.00012005735,"threshold_uncertainty_score":0.010135114},"labels":[],"label_agreement":null},{"id":"W2793765145","doi":"10.3847/1538-4357/aae51d","title":"Modeling the Radio Background from the First Black Holes at Cosmic Dawn: Implications for the 21 cm Absorption Amplitude","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":206,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Cosmic microwave background; Redshift; Halo; Amplitude; Optical depth; Black hole (networking); Planck; Approx; Absorption (acoustics); Luminosity; Galaxy; Optics","score_opus":0.03299336895299669,"score_gpt":0.26356711701770164,"score_spread":0.23057374806470493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2793765145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97949904,0.00024224872,0.016949,0.0002024977,0.000015938176,0.000008621912,0.00019592303,0.00010950707,0.002777251],"genre_scores_gemma":[0.99857974,0.000039909995,0.0011202481,0.000017583448,0.000008480749,0.0000031111636,0.00007768932,0.00001311081,0.00014021523],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998797,0.00002683108,0.0000036060753,0.000035825487,0.000021270764,0.000032842912],"domain_scores_gemma":[0.9991703,0.00040741285,0.00019375385,0.000059477516,0.000056321736,0.00011268479],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007028225,0.0005227029,0.00020679933,0.000438742,0.00021414344,0.0007917197,0.00050707144,0.00043576327,0.00069045596],"category_scores_gemma":[0.0021813274,0.00022078732,0.0003699536,0.00021946675,0.0002739381,0.0005289955,0.0005586316,0.00037564104,0.00013452682],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004888617,0.000081882084,0.64067256,0.00007593082,0.00016071735,0.00053376186,0.00019384254,0.29923925,0.019925514,0.018931214,0.00075484155,0.018941665],"study_design_scores_gemma":[0.000051014384,0.00011076971,0.21389028,0.000026889535,0.00006588354,0.00018267802,0.00008125468,0.768663,0.0066402685,0.008721013,0.0015302316,0.000036718426],"about_ca_topic_score_codex":0.004187339,"about_ca_topic_score_gemma":0.0022547771,"teacher_disagreement_score":0.004187339,"about_ca_system_score_codex":0.00058313506,"about_ca_system_score_gemma":0.00017797935,"threshold_uncertainty_score":0.008325934},"labels":[],"label_agreement":null},{"id":"W2793977486","doi":"10.1088/0004-637x/720/2/1016","title":"STELLAR POPULATIONS OF Lyα EMITTERS AT<i>z</i>= 4.86: A COMPARISON TO<i>z</i>∼ 5 LYMAN BREAK GALAXIES","year":2010,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Stellar mass; Photometry (optics); Star formation; Population; Luminosity; Stellar population; Spectral energy distribution; Astronomy; Stars","score_opus":0.022377291152625163,"score_gpt":0.30412758803660955,"score_spread":0.2817502968839844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2793977486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992931,0.000039390066,0.000036734702,0.0000039562356,3.7048383e-7,0.0000014155744,0.00017080054,0.0000026129378,0.00045165003],"genre_scores_gemma":[0.99878424,0.00004363256,0.00009484874,0.00000654324,0.0000023021823,0.0000028638997,0.00062347914,0.0000017245461,0.0004404363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998864,0.0000073447427,0.000008886706,0.000036367626,0.000015303409,0.000045655393],"domain_scores_gemma":[0.9996252,0.000038222184,0.00015114615,0.000025434354,0.00005383354,0.00010617486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001876281,0.00013917348,0.00017406218,0.001302573,0.00026181762,0.0005706281,0.00022717957,0.00019671966,0.001525426],"category_scores_gemma":[0.00026015023,0.00010478152,0.00022938159,0.0005720286,0.0002065991,0.00034266303,0.000408961,0.00014297261,0.00043407257],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012717162,0.000036975645,0.99310184,0.000009253631,0.00001890753,0.00009570432,0.00025565634,0.00013638218,0.0035092593,0.0001449979,0.00009845447,0.0024654358],"study_design_scores_gemma":[0.0000016354704,0.000016362777,0.9993705,0.0000016404346,0.0000056073036,0.00007090206,0.00014080618,0.00009100133,0.00015597227,0.00001779713,0.00012674398,0.000001009576],"about_ca_topic_score_codex":0.0047501205,"about_ca_topic_score_gemma":0.00629594,"teacher_disagreement_score":0.0047501205,"about_ca_system_score_codex":0.00028165974,"about_ca_system_score_gemma":0.000085353495,"threshold_uncertainty_score":0.009444952},"labels":[],"label_agreement":null},{"id":"W2794176654","doi":"10.3847/1538-4357/aac6b6","title":"Hidden in Plain Sight: A Massive, Dusty Starburst in a Galaxy Protocluster at z = 5.7 in the COSMOS Field","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Galaxy; Interacting galaxy; COSMIC cancer database; Stars; Galaxy merger; Star formation; Type-cD galaxy; Galaxy formation and evolution; Galaxy cluster","score_opus":0.009003625216639007,"score_gpt":0.22686506548609564,"score_spread":0.21786144026945664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794176654","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99960536,0.00003789235,0.000049548926,0.000036790814,0.000002928098,0.0000014419594,0.000025149024,0.0000045320826,0.00023632812],"genre_scores_gemma":[0.99981123,0.000019052159,0.0000532484,0.000013882622,0.000004165347,3.8157683e-7,0.00003300733,7.1675277e-7,0.00006428584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999386,0.0000065060126,0.0000029322603,0.000018045357,0.000014800268,0.000019088964],"domain_scores_gemma":[0.9996747,0.000026511532,0.00009779149,0.000024689698,0.000026425356,0.0001497828],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015615275,0.00012447544,0.00015465892,0.00049729145,0.0005044191,0.00039820207,0.00022616681,0.00019017345,0.00065895147],"category_scores_gemma":[0.00023791843,0.000075597105,0.0000931192,0.00025104792,0.0004819087,0.0002316811,0.000509576,0.00021295293,0.00013646964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001105559,0.0000398612,0.98182136,0.000007817334,0.00002381329,0.0016954935,0.0008562396,0.00007265501,0.010894024,0.00023955187,0.00024891543,0.003989671],"study_design_scores_gemma":[0.0000050757367,0.00007915593,0.996819,0.0000041382173,0.000011655587,0.0008818588,0.00070325116,0.00022691181,0.0006680226,0.000110729074,0.00048680295,0.0000033698443],"about_ca_topic_score_codex":0.0074487887,"about_ca_topic_score_gemma":0.01131216,"teacher_disagreement_score":0.0074487887,"about_ca_system_score_codex":0.00035520285,"about_ca_system_score_gemma":0.00013326552,"threshold_uncertainty_score":0.01481086},"labels":[],"label_agreement":null},{"id":"W2794324962","doi":"10.3847/1538-4357/aaca2f","title":"Accurate Determination of Halo Velocity Bias in Simulations and Its Cosmological Implications","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Halo; Physics; Redshift; Astrophysics; Galaxy; Cosmic variance; Cosmology; Sign (mathematics); Peculiar velocity; Measure (data warehouse); Amplitude; Statistics; Quantum mechanics; Mathematical analysis; Mathematics","score_opus":0.03481663558502245,"score_gpt":0.28212298805441155,"score_spread":0.2473063524693891,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794324962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94930977,0.0002479798,0.04568476,0.0003972864,0.000069561946,0.00001593119,0.00031429785,0.0008829029,0.0030775252],"genre_scores_gemma":[0.9913872,0.00003523745,0.008180039,0.000050518654,0.000007929028,0.00000824607,0.00011826814,0.00010120979,0.00011128418],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995858,0.0001741356,0.000027538064,0.00006901736,0.00009172371,0.000051740742],"domain_scores_gemma":[0.994341,0.0033162052,0.0005933815,0.0010078091,0.0005827839,0.00015876495],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016796644,0.0003221962,0.00028962633,0.0004157307,0.00035272248,0.00054467743,0.00060065713,0.00044548867,0.0007864299],"category_scores_gemma":[0.0136830155,0.0002312609,0.0002507551,0.00040135224,0.00051002187,0.000606784,0.00044660264,0.00067343755,0.00012507188],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002505501,0.00015572716,0.11018517,0.00013446558,0.00022443407,0.00019154695,0.00027491816,0.82887536,0.024906486,0.016905768,0.0019332877,0.015962292],"study_design_scores_gemma":[0.000009900258,0.000022411421,0.007724936,0.000017613673,0.000012992129,0.000024345007,0.000024964556,0.983991,0.005433124,0.002405718,0.00031749016,0.00001549096],"about_ca_topic_score_codex":0.00884055,"about_ca_topic_score_gemma":0.004455741,"teacher_disagreement_score":0.00884055,"about_ca_system_score_codex":0.00045417607,"about_ca_system_score_gemma":0.0005701654,"threshold_uncertainty_score":0.017578185},"labels":[],"label_agreement":null},{"id":"W2794340307","doi":"10.3847/1538-4357/aa9fec","title":"Nonlocal Ohms Law, Plasma Resistivity, and Reconnection During Collisions of Magnetic Flux Ropes","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Magnetic confinement fusion research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Electrical resistivity and conductivity; Magnetic reconnection; Ohm's law; Ohm; Flux (metallurgy); Plasma; Magnetic flux; Magnetohydrodynamics; Magnetic field; Condensed matter physics; Computational physics; Nuclear physics; Quantum mechanics","score_opus":0.010495000409599472,"score_gpt":0.2452269166259733,"score_spread":0.23473191621637382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794340307","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956566,0.00021050023,0.0028010504,0.00003252005,0.000007882629,0.000010577597,0.000066882574,0.00006391653,0.0011501141],"genre_scores_gemma":[0.9997938,0.0000150335545,0.000085880165,0.0000016447191,0.0000018841409,0.0000022129434,0.000017071583,0.000003217241,0.00007928631],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980026,0.00004390639,0.0000065143877,0.00004520036,0.00006112005,0.000042980693],"domain_scores_gemma":[0.99873596,0.00065079774,0.00029545318,0.00013942651,0.00010334002,0.00007498541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036631376,0.0001674829,0.00034070938,0.00058676343,0.0003107047,0.0004964936,0.0003565161,0.00028285728,0.0011088664],"category_scores_gemma":[0.0016340875,0.00016150175,0.00011027123,0.00039499882,0.0010262658,0.00060878135,0.0004734674,0.0003803143,0.00012534995],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0027556594,0.0003426286,0.082316436,0.00030301907,0.00015997354,0.0053744772,0.0022738397,0.028856538,0.8483664,0.009603594,0.0010409553,0.018606441],"study_design_scores_gemma":[0.00022873882,0.002699745,0.36668968,0.000057561276,0.000088145585,0.0037186032,0.002300965,0.23861891,0.36948928,0.013236645,0.0026835809,0.00018816626],"about_ca_topic_score_codex":0.00025983664,"about_ca_topic_score_gemma":0.00016373614,"teacher_disagreement_score":0.0011088664,"about_ca_system_score_codex":0.00019178921,"about_ca_system_score_gemma":0.00006122537,"threshold_uncertainty_score":0.003709495},"labels":[],"label_agreement":null},{"id":"W2794422641","doi":"10.3847/1538-4357/aabace","title":"Revisiting the Cooling Flow Problem in Galaxies, Groups, and Clusters of Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":135,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Cooling flow; Star formation; Accretion (finance); Magnitude (astronomy); Stars; Intracluster medium; Radiative transfer; Galaxy cluster; Astronomy","score_opus":0.007503138603123334,"score_gpt":0.2111556493734092,"score_spread":0.20365251077028587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794422641","genre_codex":"empirical","genre_gemma":"review","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"review","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987431,0.00012350471,0.00068308087,0.000045077533,0.0000017877492,0.0000050089434,0.00011900746,0.000005234171,0.00027423253],"genre_scores_gemma":[0.99939156,0.00002278123,0.00029225482,0.00000868685,0.0000071880863,0.0000035595385,0.00015433476,0.0000037932525,0.00011583097],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.998546,0.0007160429,0.00004693973,0.00028761092,0.00016330415,0.00024020232],"domain_scores_gemma":[0.9866649,0.007856855,0.0023959952,0.001625975,0.0009330384,0.00052319595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002725094,0.00024892,0.0005063897,0.0025389872,0.00088024425,0.0010750352,0.00069242355,0.00042058286,0.0013606228],"category_scores_gemma":[0.014060534,0.00015357908,0.00041398764,0.0024546224,0.0013817528,0.0010706598,0.0009296205,0.0005212141,0.00015899466],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051776045,0.000025609916,0.9903356,0.000009990354,0.000054353324,0.00004322034,0.0006606097,0.0024616604,0.00037992123,0.0010833351,0.00016603433,0.0047279615],"study_design_scores_gemma":[0.000009483631,0.000048715723,0.97892636,0.000009534433,0.00003614746,0.00015473367,0.00093997206,0.016800523,0.00038072738,0.001580184,0.0011032199,0.000010302429],"about_ca_topic_score_codex":0.025251033,"about_ca_topic_score_gemma":0.019155068,"teacher_disagreement_score":0.025251033,"about_ca_system_score_codex":0.0006594317,"about_ca_system_score_gemma":0.0004841457,"threshold_uncertainty_score":0.05020809},"labels":[],"label_agreement":null},{"id":"W2794507647","doi":"10.3847/1538-4357/aaba70","title":"The Next Generation Fornax Survey (NGFS). III. Revealing the Spatial Substructure of the Dwarf Galaxy Population Inside Half of Fornax's Virial Radius","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Fornax Cluster; Dwarf galaxy; Galaxy; RADIUS; Substructure; Population; Dwarf spheroidal galaxy; Virial theorem; Milky Way","score_opus":0.020556795295614244,"score_gpt":0.2310572228893851,"score_spread":0.21050042759377086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794507647","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9909287,0.00023388925,0.00015047747,0.000049885683,0.000005650975,0.000017559803,0.0056336196,0.000035083336,0.0029450415],"genre_scores_gemma":[0.97513914,0.00021744362,0.0013132558,0.00004516009,0.000023765264,0.000030563842,0.019774258,0.000014175304,0.003442217],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986076,0.000014762747,0.0000063870807,0.00003910368,0.000044248114,0.000034647775],"domain_scores_gemma":[0.99968886,0.000020299296,0.00009523761,0.000048699007,0.000047373054,0.00009948041],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028597697,0.00016175373,0.00016856642,0.0009683966,0.00027981025,0.00025540986,0.00022036921,0.00013825079,0.001486355],"category_scores_gemma":[0.0003591351,0.000087315544,0.00023229247,0.00041524193,0.00014944744,0.00024863632,0.00055284,0.00010617697,0.00038779725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000109316796,0.000021144344,0.9697762,0.00004430758,0.000048942115,0.00018955214,0.00041801893,0.0001413506,0.0066041094,0.00024696218,0.0031105352,0.019289574],"study_design_scores_gemma":[0.0000035000762,0.0000182842,0.9966556,0.000004649627,0.0000064567344,0.000090819056,0.00006302983,0.00011378178,0.0002753686,0.00002380197,0.002742622,0.0000019206086],"about_ca_topic_score_codex":0.025528409,"about_ca_topic_score_gemma":0.05566473,"teacher_disagreement_score":0.025528409,"about_ca_system_score_codex":0.00044993457,"about_ca_system_score_gemma":0.00032789426,"threshold_uncertainty_score":0.050759614},"labels":[],"label_agreement":null},{"id":"W2794558609","doi":"10.3847/1538-4357/aad188","title":"The CHIME Fast Radio Burst Project: System Overview","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":372,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; McGill University; University of British Columbia","funders":"","keywords":"Fast radio burst; Radio telescope; Physics; Computer science; Astronomy; Astrophysics; Galaxy","score_opus":0.018589206594299027,"score_gpt":0.3271283525471107,"score_spread":0.3085391459528117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794558609","genre_codex":"software","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17011385,0.0049146316,0.2691668,0.0044478443,0.0005078636,0.009062815,0.13828246,0.28974023,0.11376353],"genre_scores_gemma":[0.39515075,0.0014010585,0.37938827,0.001522984,0.0004120055,0.0033203035,0.18304004,0.007808782,0.027955746],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9989594,0.00009792097,0.000027014541,0.0002395716,0.00048000368,0.00019600535],"domain_scores_gemma":[0.9991235,0.00004951711,0.000046258574,0.0001607586,0.00039262234,0.00022748605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027374534,0.0010708709,0.00078790163,0.0017509802,0.0010537936,0.0028636134,0.0020489262,0.001148109,0.014023419],"category_scores_gemma":[0.0012926358,0.0007370973,0.00039120737,0.002027062,0.00053271273,0.0014450421,0.0021190192,0.00091225596,0.010046709],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.003321882,0.00070288905,0.06507789,0.0009733933,0.00042107393,0.00066443277,0.0009365814,0.020642316,0.07781044,0.009893389,0.46666932,0.35288632],"study_design_scores_gemma":[0.0010678641,0.0011962894,0.09401227,0.00025382108,0.00021107496,0.0008606485,0.00043173027,0.17689317,0.05626608,0.0063476334,0.6618558,0.00060357637],"about_ca_topic_score_codex":0.054668225,"about_ca_topic_score_gemma":0.039771043,"teacher_disagreement_score":0.054668225,"about_ca_system_score_codex":0.0022235666,"about_ca_system_score_gemma":0.0031463096,"threshold_uncertainty_score":0.10870004},"labels":[],"label_agreement":null},{"id":"W2794648399","doi":"10.3847/1538-4357/aabad8","title":"Dense Gas, Dynamical Equilibrium Pressure, and Star Formation in Nearby Star-forming Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Star formation; Galaxy; Galaxy formation and evolution; Stellar evolution; Young stellar object; Range (aeronautics); Stars","score_opus":0.009715013478532722,"score_gpt":0.2368439591289167,"score_spread":0.227128945650384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794648399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997727,0.000014975057,0.00005653522,0.0000037967409,2.3377828e-7,7.924048e-7,0.000046446898,0.000003508546,0.00010098486],"genre_scores_gemma":[0.9998356,0.000005602044,0.000057221932,0.000001842987,0.0000010479104,8.170674e-7,0.00006554023,6.350002e-7,0.000031639946],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998764,0.000027745018,0.0000073158258,0.000035422243,0.000031005573,0.000022208527],"domain_scores_gemma":[0.9988752,0.00028282744,0.0003547353,0.0001438122,0.0000958047,0.00024759577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030072444,0.00011756464,0.00017851165,0.0009588151,0.00023338427,0.00044853127,0.0002116368,0.00016378501,0.0006740119],"category_scores_gemma":[0.001240452,0.00012081023,0.00012397449,0.00048714032,0.00036927476,0.00033139327,0.00043212553,0.00014777265,0.00007563706],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005979409,0.000020549693,0.9942801,0.0000035284318,0.000024477367,0.000026839323,0.000123913,0.00022748725,0.004016551,0.000041008338,0.000015485972,0.0011602994],"study_design_scores_gemma":[0.0000015373903,0.0000205261,0.9993722,4.825338e-7,0.0000032434696,0.000020178119,0.000049851915,0.0002933152,0.00018226118,0.00002549277,0.000029954037,0.0000011600227],"about_ca_topic_score_codex":0.0068637514,"about_ca_topic_score_gemma":0.00914866,"teacher_disagreement_score":0.0068637514,"about_ca_system_score_codex":0.00028209592,"about_ca_system_score_gemma":0.00007066487,"threshold_uncertainty_score":0.013647556},"labels":[],"label_agreement":null},{"id":"W2794668368","doi":"10.3847/1538-4357/ab1754","title":"Optical Properties of Infrared-bright Dust-obscured Galaxies Viewed with Subaru Hyper Suprime-Cam","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Japan Society for the Promotion of Science; Science Mission Directorate; University of California, Los Angeles; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; Space Telescope Science Institute; Astronomical Society of Japan; Princeton University; Johns Hopkins University; Jet Propulsion Laboratory; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; Academia Sinica; California Institute of Technology; Durham University; Japan Science and Technology Agency; Smithsonian Institution; National Science Foundation","keywords":"Galaxy; Supermassive black hole; Infrared; Active galactic nucleus; Star formation; Near-infrared spectroscopy; Subaru Telescope; Luminous infrared galaxy","score_opus":0.007309485018534297,"score_gpt":0.18537084599795745,"score_spread":0.17806136097942316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794668368","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998871,0.00005597032,0.00008149685,0.000006016056,0.0000018568817,0.0000033524782,0.00027715525,0.000014750355,0.00068823557],"genre_scores_gemma":[0.9986689,0.00003847311,0.0003306933,0.000015606305,0.00000887201,0.0000045514494,0.0007459818,0.0000054461716,0.00018142321],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990773,0.000009406776,0.000005723209,0.000025774552,0.00002435357,0.00002708419],"domain_scores_gemma":[0.9996032,0.00004273894,0.00013027959,0.000035569887,0.000053267384,0.00013496219],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020849588,0.00024516977,0.00022774063,0.0015181943,0.00028696185,0.00043658674,0.00023160316,0.00017642556,0.00087347627],"category_scores_gemma":[0.00025171757,0.00015086432,0.0001793904,0.0006978555,0.00020744314,0.00022488268,0.00043159735,0.0001390085,0.00023126863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017756704,0.00004749541,0.9735693,0.000022155686,0.00004967982,0.0002545498,0.00038391954,0.00010678297,0.01939001,0.000058913996,0.0003452129,0.0055945134],"study_design_scores_gemma":[0.0000015504581,0.000017421942,0.999099,0.0000016207496,0.000009409266,0.00006705156,0.00008961828,0.00010215995,0.00043883215,0.0000056351378,0.0001664786,0.0000012030785],"about_ca_topic_score_codex":0.002656711,"about_ca_topic_score_gemma":0.0052141934,"teacher_disagreement_score":0.002656711,"about_ca_system_score_codex":0.00014742742,"about_ca_system_score_gemma":0.000056550653,"threshold_uncertainty_score":0.0052824616},"labels":[],"label_agreement":null},{"id":"W2794857586","doi":"10.3847/1538-4357/aac025","title":"A Holistic Perspective on the Dynamics of G035.39-00.33: The Interplay between Gas and Magnetic Fields","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Waterloo; Herzberg Institute of Astrophysics","funders":"East Asian Core Observatories Association; National Astronomical Observatory of Japan; Jet Propulsion Laboratory; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; Hungarian Scientific Research Fund; Chinese Academy of Sciences; California Institute of Technology; Academia Sinica; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; National Natural Science Foundation of China","keywords":"Magnetic field; Polarization (electrochemistry); Star formation; Molecular cloud; Accretion (finance); Gravitational collapse; Field line; Perpendicular; Gravitation; Magnetic pressure","score_opus":0.011773590510519783,"score_gpt":0.276393259420596,"score_spread":0.2646196689100762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2794857586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87795746,0.02613063,0.022169085,0.022716047,0.00045259748,0.00002464807,0.001976513,0.00031567723,0.048257396],"genre_scores_gemma":[0.9920533,0.0033695898,0.0024574199,0.0006207509,0.00014435456,0.0000057810425,0.0002666066,0.000034621247,0.0010475328],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995875,0.000006310862,0.0000013093199,0.000012407042,0.00000638023,0.000014837296],"domain_scores_gemma":[0.9999236,0.000009365311,0.000016254142,0.0000086144,0.000016678934,0.000025563357],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014455605,0.00019316364,0.00028139885,0.00049765874,0.000386255,0.0011958367,0.00031876718,0.00043959793,0.0018863056],"category_scores_gemma":[0.00017609935,0.000077338285,0.000147112,0.00042332933,0.0005969091,0.0011614314,0.0005834172,0.000478776,0.00022751969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037582198,0.00016105047,0.26108673,0.000789648,0.0003429492,0.003654162,0.0038832359,0.03262931,0.24129294,0.2586503,0.030024305,0.16710956],"study_design_scores_gemma":[0.00001877993,0.00018013806,0.6205685,0.00044809282,0.00016879659,0.0012928596,0.006674052,0.043298267,0.008550411,0.21299851,0.1056468,0.00015478897],"about_ca_topic_score_codex":0.002666101,"about_ca_topic_score_gemma":0.0037605069,"teacher_disagreement_score":0.002666101,"about_ca_system_score_codex":0.00063992443,"about_ca_system_score_gemma":0.00021531289,"threshold_uncertainty_score":0.0063103437},"labels":[],"label_agreement":null},{"id":"W2795266307","doi":"10.1086/309451","title":"Scattering and Diffraction in Magnetospheres of Fast Pulsars","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Pulsar; Physics; Scattering; Magnetosphere; Computational physics; Radio wave; Diffraction; Forward scatter; Astrophysics; Optics; Plasma; Quantum mechanics","score_opus":0.007206507623198655,"score_gpt":0.2821824895647514,"score_spread":0.27497598194155276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795266307","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9689053,0.0012231236,0.026769709,0.000100136655,0.000027887441,0.000009959061,0.000041262865,0.00005230182,0.0028702796],"genre_scores_gemma":[0.99524,0.0006565532,0.0032773016,0.000013254407,0.000020841533,0.000007262227,0.00006546516,0.000011657473,0.00070766127],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987626,0.000026034118,0.000005509639,0.00001630459,0.000043431457,0.000032540724],"domain_scores_gemma":[0.99953353,0.00021936627,0.00013199364,0.00003953674,0.000042214713,0.000033323988],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034812323,0.00035206636,0.0002136393,0.0007359683,0.00051976764,0.00069570437,0.00017562212,0.00024930644,0.000427922],"category_scores_gemma":[0.0013312744,0.00022814747,0.00033325274,0.00068037014,0.0006291095,0.0005433832,0.0008226337,0.00031943494,0.00009499231],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007974181,0.00013089059,0.10314323,0.00031465085,0.00024719074,0.0018701246,0.0031903416,0.37801942,0.3002392,0.13476205,0.00095858646,0.07632677],"study_design_scores_gemma":[0.0001307356,0.00053927285,0.13127227,0.000044290868,0.000090439586,0.0018950478,0.00095472275,0.7146826,0.044287305,0.101696104,0.0042554187,0.00015179993],"about_ca_topic_score_codex":0.0027326623,"about_ca_topic_score_gemma":0.0011637233,"teacher_disagreement_score":0.0027326623,"about_ca_system_score_codex":0.00042333273,"about_ca_system_score_gemma":0.0003005338,"threshold_uncertainty_score":0.00543344},"labels":[],"label_agreement":null},{"id":"W2795411121","doi":"10.3847/1538-4357/aab668","title":"Applying a Particle-only Model to the HL Tau Disk","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Planet; Simple (philosophy); Planetary system; Star (game theory); Jupiter (rocket family); Debris disk; Celestial mechanics; Protoplanetary disk","score_opus":0.018953613993544,"score_gpt":0.26304549531103244,"score_spread":0.24409188131748843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795411121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96661913,0.0003034241,0.020218275,0.00079112273,0.00009406878,0.00010262713,0.0005664381,0.00016284005,0.011141994],"genre_scores_gemma":[0.99609756,0.0000954312,0.002105753,0.00006981004,0.000024460307,0.000040668223,0.00011064513,0.000025699514,0.0014300641],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998857,0.000036576712,0.000005925659,0.000025044501,0.0000180773,0.00002858852],"domain_scores_gemma":[0.99943715,0.0002332842,0.00008857569,0.000051959454,0.000090703106,0.000098373566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027554878,0.00056986033,0.0008622466,0.0004921155,0.0009127885,0.0011188032,0.0014719316,0.0020494333,0.00211608],"category_scores_gemma":[0.0014502689,0.00034961072,0.0008479757,0.00031531454,0.00077799446,0.0010868214,0.00079653563,0.00067523576,0.0002944396],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050405397,0.000050643666,0.0032494257,0.000021756014,0.000021851392,0.00020170832,0.000056539295,0.9926923,0.0009636442,0.0017031692,0.00019814432,0.00079034833],"study_design_scores_gemma":[0.00003527831,0.00002225253,0.0006168427,0.0000027213598,0.000008291076,0.000014092395,0.000019992003,0.9985819,0.00010695312,0.00043316284,0.00015320431,0.000005415643],"about_ca_topic_score_codex":0.04556519,"about_ca_topic_score_gemma":0.0135477595,"teacher_disagreement_score":0.04556519,"about_ca_system_score_codex":0.0011583257,"about_ca_system_score_gemma":0.00076969404,"threshold_uncertainty_score":0.090599954},"labels":[],"label_agreement":null},{"id":"W2795425373","doi":"10.3847/1538-4357/aab606","title":"Seeing Red in NGC 1978, NGC 55, and NGC 3109*<sup>†</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Astrophysics; Stars; Galaxy; Spectral line; Astronomy; Hubble sequence; Dwarf galaxy; Star cluster; Spiral galaxy","score_opus":0.010237032328935889,"score_gpt":0.2245518285683039,"score_spread":0.21431479623936803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795425373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974975,0.000022902868,0.00003767631,0.000009874951,0.0000022348238,0.0000011836369,0.0003969761,0.000015538913,0.002016162],"genre_scores_gemma":[0.9982486,0.000014011279,0.00012697242,0.0000067059723,0.0000020721027,0.0000018686034,0.0010485764,0.000005785829,0.000545495],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999323,0.000003306815,0.000002112103,0.000019755926,0.000016346825,0.00002617205],"domain_scores_gemma":[0.99974495,0.000032173466,0.000050738287,0.000017128803,0.000063395826,0.00009156578],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000060670027,0.00014683284,0.00009049587,0.0006589715,0.00027682722,0.0002526729,0.00013304841,0.00013312315,0.0023832924],"category_scores_gemma":[0.00017023855,0.00007288874,0.00009215694,0.0003728262,0.00014903588,0.00009934921,0.00014894055,0.00009628954,0.00040876886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030808724,0.00003262068,0.9488549,0.000024812669,0.000022384718,0.0003836578,0.0006777257,0.00036230526,0.038512316,0.00029227286,0.0017867525,0.00874221],"study_design_scores_gemma":[9.239433e-7,0.0000057447255,0.9990792,9.913541e-7,0.0000031568447,0.00002495845,0.00010729855,0.00007434288,0.0003560623,0.0000064313954,0.000340106,6.48019e-7],"about_ca_topic_score_codex":0.06539328,"about_ca_topic_score_gemma":0.16635865,"teacher_disagreement_score":0.06539328,"about_ca_system_score_codex":0.000648648,"about_ca_system_score_gemma":0.00012447804,"threshold_uncertainty_score":0.13002527},"labels":[],"label_agreement":null},{"id":"W2795587333","doi":"10.3847/1538-4357/aab35a","title":"Revival of the Magnetar PSR J1622–4950: Observations with MeerKAT, Parkes, XMM-Newton, Swift, Chandra, and NuSTAR","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":160,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"Goddard Space Flight Center; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory","keywords":"Magnetar; Physics; Astrophysics; Pulsar; Neutron star; Flux (metallurgy); Magnetosphere; Swift; Astronomy; Millisecond pulsar; Magnetic field","score_opus":0.014702338490143256,"score_gpt":0.2746993942509728,"score_spread":0.25999705576082954,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795587333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984251,0.00022265881,0.00013839683,0.000058397727,0.000015170384,0.000006578164,0.00015203255,0.000024626783,0.0009571109],"genre_scores_gemma":[0.9991781,0.00007772994,0.00011725728,0.000043853048,0.00002096429,0.000005080553,0.00029594277,0.000008174982,0.00025286037],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998273,0.000017576545,0.000013135305,0.00005031653,0.000047906622,0.00004380674],"domain_scores_gemma":[0.9994056,0.000043049033,0.00020751357,0.000083955165,0.000087049564,0.00017279496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043517773,0.00023113965,0.00032973627,0.0008096722,0.00047264536,0.0008035256,0.0003376313,0.00034192734,0.0006071253],"category_scores_gemma":[0.0006130058,0.00022174406,0.00017570335,0.00044654665,0.00045928705,0.0003961554,0.0007173592,0.0005456702,0.00041361823],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003618113,0.000102203754,0.89538205,0.000055674736,0.00014541093,0.0015672175,0.00089439016,0.0002154049,0.08331339,0.0002382617,0.0013344466,0.016389806],"study_design_scores_gemma":[0.000009568073,0.00007838038,0.9963225,0.000008928756,0.00001772119,0.00039206192,0.00013992323,0.00017627835,0.001352359,0.00003134535,0.0014635852,0.0000073195197],"about_ca_topic_score_codex":0.0042183893,"about_ca_topic_score_gemma":0.009548652,"teacher_disagreement_score":0.0042183893,"about_ca_system_score_codex":0.0003657075,"about_ca_system_score_gemma":0.00018608358,"threshold_uncertainty_score":0.008387685},"labels":[],"label_agreement":null},{"id":"W2795624267","doi":"10.3847/1538-4357/aac6ed","title":"A New Look at an Old Cluster: The Membership, Rotation, and Magnetic Activity of Low-mass Stars in the 1.3 Gyr Old Open Cluster NGC 752","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Open cluster; Stars; Photometry (optics); Cluster (spacecraft); Star cluster; Stellar rotation; Stellar evolution; Starspot","score_opus":0.01385530971413352,"score_gpt":0.24836055113797834,"score_spread":0.23450524142384482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795624267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980574,0.00015193858,0.000157953,0.00005939359,0.000004439193,0.000002373212,0.00031625826,0.000011267156,0.0012388756],"genre_scores_gemma":[0.99876297,0.000058304613,0.00025637058,0.000017737055,0.000017686683,0.0000019160568,0.00036137967,0.0000049002006,0.0005187755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993634,0.000006148463,0.000003879237,0.000019559686,0.000018669645,0.000015327265],"domain_scores_gemma":[0.9996556,0.00003582504,0.000066132445,0.000033210825,0.00006172251,0.00014754997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023589053,0.00018550323,0.0001805239,0.0019461449,0.00067623524,0.0007661369,0.00023733299,0.00023419477,0.0017061554],"category_scores_gemma":[0.00045477867,0.00006734878,0.00013265936,0.0010434153,0.00034673273,0.0006217773,0.00049856346,0.00021003606,0.00028828907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007903596,0.00002914747,0.9799754,0.00001566639,0.000018983957,0.0002788353,0.0011042389,0.00019896809,0.0106984,0.00018452258,0.0005412451,0.006875498],"study_design_scores_gemma":[6.457127e-7,0.00001347027,0.9987338,0.000002183643,0.00000500585,0.00007676326,0.00033799966,0.0000868638,0.0001757239,0.000031147716,0.0005340585,0.0000023807977],"about_ca_topic_score_codex":0.02278971,"about_ca_topic_score_gemma":0.06318855,"teacher_disagreement_score":0.02278971,"about_ca_system_score_codex":0.0005698261,"about_ca_system_score_gemma":0.00020584013,"threshold_uncertainty_score":0.045314133},"labels":[],"label_agreement":null},{"id":"W2795690500","doi":"10.3847/1538-4357/aac2b8","title":"BANYAN. XII. New Members of Nearby Young Associations from GAIA–Tycho Data","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Association (psychology); Radial velocity; Trigonometry; Bayesian probability; Kinematics; Survey data collection","score_opus":0.02678095677845455,"score_gpt":0.26424233498435845,"score_spread":0.2374613782059039,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795690500","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9840671,0.00048248674,0.0025199428,0.000036195306,0.000021073189,0.000046430774,0.0050943024,0.0002609775,0.007471494],"genre_scores_gemma":[0.96567285,0.0003252828,0.0076066265,0.00006297646,0.000031127183,0.00006585893,0.022019004,0.00017966726,0.004036529],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996952,0.000024171124,0.000022445853,0.00007728566,0.00012159866,0.00005943106],"domain_scores_gemma":[0.99888915,0.0000944333,0.00039247633,0.0002210941,0.00018116648,0.00022171975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005241832,0.0002087117,0.0002824711,0.0032394484,0.0008152351,0.0010581259,0.00039219187,0.00015666848,0.0036920917],"category_scores_gemma":[0.00089137594,0.00016163486,0.00022272981,0.003288744,0.00020423059,0.00031016013,0.0011192535,0.0002673265,0.0018723123],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022501363,0.00003812163,0.93438065,0.00008638632,0.00006690191,0.00032902585,0.0008732105,0.0004886237,0.016231239,0.00045803643,0.002342157,0.04448071],"study_design_scores_gemma":[0.000010981012,0.000027463962,0.97676533,0.000018065477,0.0000368874,0.00040134578,0.00031482292,0.0011620986,0.002408317,0.00018923207,0.018653644,0.000011836946],"about_ca_topic_score_codex":0.015822185,"about_ca_topic_score_gemma":0.037149217,"teacher_disagreement_score":0.015822185,"about_ca_system_score_codex":0.00029170053,"about_ca_system_score_gemma":0.00041776992,"threshold_uncertainty_score":0.031460166},"labels":[],"label_agreement":null},{"id":"W2795760988","doi":"10.3847/1538-4357/aac9bc","title":"The Dispersion and Rotation Measure of Supernova Remnants and Magnetized Stellar Winds: Application to Fast Radio Bursts","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":89,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Supernova; Astrophysics; Ejecta; Neutron star; Interstellar medium; Galaxy; Ionization; Supernova remnant; Stars; Compact star; Astronomy; Ion","score_opus":0.007409785065920415,"score_gpt":0.2792616256330074,"score_spread":0.27185184056708694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795760988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900669,0.0005078676,0.0069297156,0.000054343764,0.000012954007,0.00000901935,0.00049879175,0.00010847355,0.0018119314],"genre_scores_gemma":[0.99739456,0.000076478136,0.002208291,0.000004471576,0.000015452417,0.0000027911537,0.00017822988,0.000008565842,0.00011113174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999821,0.0000607764,0.000017380578,0.000046839792,0.000036011916,0.000017977982],"domain_scores_gemma":[0.9971641,0.0010202343,0.0011185245,0.00030958955,0.0001905544,0.00019701319],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000537501,0.00025054626,0.00016716444,0.002317182,0.00013642514,0.00046966702,0.00018816379,0.00018358578,0.0006858481],"category_scores_gemma":[0.00415092,0.00011156146,0.00019199048,0.001282802,0.00029258514,0.00036389125,0.00043583807,0.00022920471,0.0001372872],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020183422,0.000024648121,0.9405592,0.00004368503,0.00013665594,0.00017879784,0.00016551637,0.011276273,0.011773533,0.0017348572,0.00031593646,0.03358904],"study_design_scores_gemma":[0.000011439298,0.00007740308,0.961093,0.00001705852,0.000019523362,0.00037236308,0.00013422019,0.03230394,0.0029244467,0.0019189484,0.0010945967,0.000033086188],"about_ca_topic_score_codex":0.002570873,"about_ca_topic_score_gemma":0.0016547746,"teacher_disagreement_score":0.002570873,"about_ca_system_score_codex":0.00021210204,"about_ca_system_score_gemma":0.00008647144,"threshold_uncertainty_score":0.0051118135},"labels":[],"label_agreement":null},{"id":"W2795769346","doi":"10.3847/1538-4357/aabd7d","title":"Exploring the Atmosphere of Neoproterozoic Earth: The Effect of O<sub>2</sub> on Haze Formation and Composition","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Haze; Nucleation; Particle (ecology); Nitrogen; Radiative transfer; Aerosol; Atmosphere (unit); Chemical composition; Scattering","score_opus":0.015179623234377267,"score_gpt":0.19927114447394956,"score_spread":0.1840915212395723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795769346","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988808,0.00017390659,0.00032310316,0.00002654485,0.000002758776,0.000006689339,0.00009053563,0.000007385157,0.00048821612],"genre_scores_gemma":[0.99902844,0.00014782997,0.0005766409,0.000030498875,0.000002235472,0.0000041610097,0.000066786524,0.0000049753676,0.00013833621],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999355,0.0000065396953,0.000002877226,0.000021538179,0.000020314219,0.000013294063],"domain_scores_gemma":[0.99993324,0.00002087372,0.000016240541,0.000003985894,0.000016245684,0.000009445094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021125456,0.0003651607,0.00018288693,0.00019374983,0.00028337067,0.00032603863,0.00023931943,0.00043405703,0.00048750432],"category_scores_gemma":[0.00014884898,0.00021730187,0.00014353238,0.000117729986,0.00039236163,0.00034188057,0.00022947062,0.00027585792,0.000070086244],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006266536,0.000012076594,0.011696751,0.000049870498,0.000012061803,0.00006770522,0.000057652625,0.0004028917,0.98676586,0.000050731407,0.000014845315,0.00080672913],"study_design_scores_gemma":[0.000024600944,0.00023382931,0.37044403,0.00001870631,0.000052019837,0.00013484275,0.0004644895,0.0066268644,0.6199547,0.0003128981,0.001714603,0.000018386672],"about_ca_topic_score_codex":0.004637838,"about_ca_topic_score_gemma":0.005073753,"teacher_disagreement_score":0.004637838,"about_ca_system_score_codex":0.00040238854,"about_ca_system_score_gemma":0.00019489229,"threshold_uncertainty_score":0.009221673},"labels":[],"label_agreement":null},{"id":"W2795807040","doi":"10.3847/1538-4357/aabc55","title":"Spatially Resolved Stellar Kinematics from LEGA-C: Increased Rotational Support in z ∼ 0.8 Quiescent Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Velocity dispersion; Galaxy; Redshift; Stellar population; Star formation; Elliptical galaxy; Galaxy rotation curve; Astronomy; Galaxy formation and evolution","score_opus":0.009308217132938282,"score_gpt":0.22094588077386246,"score_spread":0.21163766364092418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795807040","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972761,0.000056030316,0.00007339411,0.000029113558,0.0000018388985,0.0000030518036,0.0014942765,0.00002703239,0.0010392364],"genre_scores_gemma":[0.99586403,0.000021462678,0.00011735889,0.000027336077,0.0000047891353,0.0000035270393,0.0035013128,0.000011515082,0.00044859864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987173,0.000014074056,0.0000073427373,0.000035347737,0.0000241777,0.000047288773],"domain_scores_gemma":[0.9990682,0.00010623042,0.00029633776,0.00010411356,0.00013038085,0.0002947144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019209302,0.00018867507,0.0001947201,0.0016317058,0.00027835535,0.00080189866,0.00020105955,0.00022348498,0.002052707],"category_scores_gemma":[0.00076295924,0.00009269758,0.00018102204,0.0008430001,0.00027125518,0.00021213117,0.0006515585,0.00016648712,0.00088784005],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023589295,0.000046748537,0.9745594,0.000016077813,0.00002826007,0.00014465023,0.000439504,0.00025279107,0.015649075,0.00014358918,0.00095925375,0.007524701],"study_design_scores_gemma":[0.0000029795276,0.000013778945,0.9989341,0.0000019558283,0.0000035848705,0.000059310933,0.000053741558,0.00015141474,0.0002950888,0.000026706775,0.00045459662,0.0000027754727],"about_ca_topic_score_codex":0.010050542,"about_ca_topic_score_gemma":0.012974196,"teacher_disagreement_score":0.010050542,"about_ca_system_score_codex":0.0004011096,"about_ca_system_score_gemma":0.000110272806,"threshold_uncertainty_score":0.019984066},"labels":[],"label_agreement":null},{"id":"W2795860007","doi":"10.3847/1538-4357/aab5b9","title":"Photodissociation of CS from Excited Rovibrational Levels","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Smithsonian Astrophysical Observatory; Institute for Theoretical Atomic, Molecular and Optical Physics, Harvard University; Queen's University; Universität Stuttgart; National Aeronautics and Space Administration; Queen's University Belfast; National Energy Research Scientific Computing Center; Smithsonian Institution; National Science Foundation","keywords":"Rotational–vibrational spectroscopy; Photodissociation; Excited state; Ground state; Dipole; Diatomic molecule; Ab initio","score_opus":0.015780380341465432,"score_gpt":0.2503997375140674,"score_spread":0.234619357172602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2795860007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97263813,0.0003428737,0.020651987,0.00007503036,0.000019262978,0.00002128617,0.00025878826,0.00017966866,0.005812971],"genre_scores_gemma":[0.9973253,0.000114886156,0.0013689112,0.000011043651,0.000002106753,0.0000105839545,0.00018116269,0.000027530503,0.00095843105],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998105,0.000024975505,0.0000077454215,0.000031166102,0.00006381436,0.00006190606],"domain_scores_gemma":[0.999438,0.00024407156,0.000073164716,0.000080354424,0.00012897608,0.00003540894],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048078803,0.00038977756,0.00048078824,0.00094526913,0.0007741647,0.0007340477,0.0008764948,0.00047796182,0.003428483],"category_scores_gemma":[0.0011188575,0.00024715063,0.0005972306,0.0011484409,0.0005591726,0.0005884054,0.00045147756,0.00051688484,0.00027183382],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024795215,0.00008126034,0.011775525,0.00021477694,0.000119794844,0.00047209195,0.00027222245,0.87661016,0.054990694,0.042482417,0.00048802188,0.012245129],"study_design_scores_gemma":[0.00006888975,0.00018523424,0.011771219,0.00003696402,0.000049559785,0.00023310613,0.00017631351,0.869814,0.10704897,0.008860085,0.0016946504,0.000061001396],"about_ca_topic_score_codex":0.0070686233,"about_ca_topic_score_gemma":0.0050316784,"teacher_disagreement_score":0.0070686233,"about_ca_system_score_codex":0.0017996347,"about_ca_system_score_gemma":0.00087057357,"threshold_uncertainty_score":0.014054954},"labels":[],"label_agreement":null},{"id":"W2796002233","doi":"10.3847/1538-4357/aab895","title":"Stellar Mass and 3.4 μm M/L Ratio Evolution of Brightest Cluster Galaxies in COSMOS since z ∼ 1.0","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Stellar mass; Star formation; Galaxy; Redshift; Galaxy formation and evolution; Brightest cluster galaxy; Stellar density; Galaxy cluster","score_opus":0.005722510043375957,"score_gpt":0.20438926088725778,"score_spread":0.19866675084388183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2796002233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992205,0.00006209195,0.000049144266,0.000020976819,0.0000018206066,0.0000010607115,0.00035241857,0.000012970993,0.00027907145],"genre_scores_gemma":[0.9992244,0.000023002549,0.000068251735,0.000008202061,0.0000037827533,0.000001216258,0.00052627356,0.000004153234,0.0001407178],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989736,0.000013238926,0.0000050004537,0.000038725157,0.000013939395,0.000031698986],"domain_scores_gemma":[0.99865025,0.00013494104,0.00059146644,0.00010925015,0.00016905542,0.00034507224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005259559,0.00015829518,0.00016713353,0.0013008069,0.00021509313,0.00053087017,0.00022963343,0.00025523873,0.0014260664],"category_scores_gemma":[0.0011604545,0.000114377755,0.0002711135,0.0005598545,0.00026339522,0.00031195546,0.00040223153,0.00028947118,0.00040727443],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003969276,0.000010378123,0.99681085,0.000003925223,0.000015651603,0.000019932486,0.000085990294,0.000120110984,0.0012206938,0.000058011905,0.00012830393,0.0014863721],"study_design_scores_gemma":[7.286108e-7,0.00000721719,0.999647,8.533642e-7,0.0000027322242,0.000010407929,0.000020634721,0.000115612565,0.000105908475,0.000008908276,0.0000791095,8.947872e-7],"about_ca_topic_score_codex":0.008822897,"about_ca_topic_score_gemma":0.0087761255,"teacher_disagreement_score":0.008822897,"about_ca_system_score_codex":0.00031165284,"about_ca_system_score_gemma":0.000119784156,"threshold_uncertainty_score":0.017543077},"labels":[],"label_agreement":null},{"id":"W2796172159","doi":"10.3847/1538-4357/aab4fa","title":"A Near-infrared RR Lyrae Census along the Southern Galactic Plane: The Milky Way’s Stellar Fossil Brought to Light","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Mount Saint Vincent University","funders":"","keywords":"Milky Way; RR Lyrae variable; Galactic halo; Bulge; Metallicity; Extinction (optical mineralogy); Stars; Red clump; Galaxy","score_opus":0.011795092766368984,"score_gpt":0.2244148844903594,"score_spread":0.21261979172399043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2796172159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99891686,0.00003595037,0.00023679863,0.000009161763,6.9642635e-7,0.0000021360397,0.00063831237,0.000009381586,0.00015068699],"genre_scores_gemma":[0.99533206,0.0000451631,0.00069019326,0.000007724152,0.00000477272,0.0000043503132,0.0036813465,0.000006208597,0.00022817795],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997329,0.000040486837,0.000017439548,0.00010314706,0.000064654916,0.000041345298],"domain_scores_gemma":[0.99925727,0.000090682624,0.0002261584,0.00014632245,0.00015317097,0.00012627867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003137256,0.00012970738,0.00022300902,0.0014807042,0.00021365967,0.00045537102,0.00028467993,0.00020069222,0.0004683087],"category_scores_gemma":[0.0010668422,0.000105917694,0.00018982615,0.0010965191,0.00018118473,0.00024604087,0.00059340696,0.0001765373,0.0003097795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004838918,0.000021582611,0.9844253,0.000014610559,0.000030153225,0.00014053525,0.000244593,0.0011362645,0.0039719506,0.00016528256,0.00043726928,0.009364086],"study_design_scores_gemma":[0.0000031082254,0.000019832678,0.9947314,0.0000035524272,0.000007929292,0.00010394287,0.00016595978,0.0027523842,0.00067346083,0.00004465908,0.0014898625,0.000003835131],"about_ca_topic_score_codex":0.010392442,"about_ca_topic_score_gemma":0.012504711,"teacher_disagreement_score":0.010392442,"about_ca_system_score_codex":0.0002492722,"about_ca_system_score_gemma":0.00017909285,"threshold_uncertainty_score":0.020663857},"labels":[],"label_agreement":null},{"id":"W2796338474","doi":"10.3847/1538-4357/aabafb","title":"Flux Relaxation after Two Outbursts of the Magnetar SGR 1627–41 and Possible Hard X-Ray Emission","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Flux (metallurgy); Relaxation (psychology); Crust; Energy flux; Thermal emission","score_opus":0.009215383191509122,"score_gpt":0.29130084591182914,"score_spread":0.28208546272032003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2796338474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993734,0.00010034387,0.000083147934,0.000028039889,0.000006622329,0.0000033770589,0.00009426595,0.000012829482,0.00029791644],"genre_scores_gemma":[0.998938,0.00004251433,0.00010379111,0.000023467675,0.000013395743,0.000005426127,0.00065467757,0.0000076080273,0.00021111788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998666,0.000016602415,0.00000997111,0.000040277693,0.000029283732,0.000037148533],"domain_scores_gemma":[0.9988707,0.00021191592,0.000384537,0.00012501168,0.0001244526,0.000283501],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055038155,0.00031239953,0.00063308526,0.0007312218,0.0006703026,0.00052034017,0.0003174976,0.00051678874,0.00072423543],"category_scores_gemma":[0.001091307,0.00018058262,0.00039231376,0.0003221707,0.00035363273,0.00028945185,0.0006900221,0.0006099702,0.00026298294],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015457473,0.0003455626,0.9029379,0.0001109123,0.00022338484,0.003396573,0.0012009864,0.0007938675,0.07208373,0.0001792898,0.0006643064,0.016517652],"study_design_scores_gemma":[0.0000075480543,0.00010357876,0.99731076,0.000005099458,0.000021771997,0.00016646978,0.00008930367,0.0003366501,0.0015498301,0.000027444567,0.00037406906,0.000007552022],"about_ca_topic_score_codex":0.0031516787,"about_ca_topic_score_gemma":0.0045851823,"teacher_disagreement_score":0.0031516787,"about_ca_system_score_codex":0.0005093087,"about_ca_system_score_gemma":0.000121069716,"threshold_uncertainty_score":0.0062666535},"labels":[],"label_agreement":null},{"id":"W2796801433","doi":"10.3847/1538-4357/aabc53","title":"Difference in Dwarf Galaxy Surface Brightness Profiles as a Function of Environment*","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Virgo Cluster; Gravitational microlensing; Surface brightness; Dwarf galaxy; Brown dwarf; Galaxy; Supernova; Type (biology); Galaxy cluster","score_opus":0.0071336189372014115,"score_gpt":0.20103412966951226,"score_spread":0.19390051073231085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2796801433","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995995,0.000011829823,0.000099480436,0.0000020424286,3.3382742e-7,4.7485602e-7,0.0000711192,0.000006953174,0.00020823408],"genre_scores_gemma":[0.999658,0.000008024754,0.000055646604,0.000001764298,6.8355683e-7,6.864783e-7,0.00017322355,0.0000033418416,0.000098584096],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998734,0.000016036325,0.0000063974094,0.00004862571,0.000022364464,0.00003305216],"domain_scores_gemma":[0.99941707,0.000097193086,0.0001597542,0.00006421559,0.00009521381,0.00016655112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016923058,0.0001455465,0.00018168573,0.00061931426,0.0001502728,0.00030132453,0.00012730643,0.00011839997,0.0007326294],"category_scores_gemma":[0.0005986893,0.000089929476,0.0001530633,0.00040843192,0.00017951702,0.00024959183,0.00028509714,0.000087036555,0.00019972265],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014724485,0.000019712192,0.97392094,0.000007645174,0.00003304652,0.00009966097,0.00017167875,0.00036207915,0.021714818,0.000073951436,0.00007827927,0.0033709314],"study_design_scores_gemma":[8.359244e-7,0.000014180573,0.9987073,4.050861e-7,0.0000040921846,0.000050992185,0.000075479235,0.00031669546,0.0007329173,0.000021917958,0.00007312274,0.0000019984343],"about_ca_topic_score_codex":0.0028740866,"about_ca_topic_score_gemma":0.0030629756,"teacher_disagreement_score":0.0028740866,"about_ca_system_score_codex":0.00017556219,"about_ca_system_score_gemma":0.00007225613,"threshold_uncertainty_score":0.0057147145},"labels":[],"label_agreement":null},{"id":"W2797165970","doi":"10.3847/1538-4357/aabb56","title":"The Peculiar Radial Distribution of Multiple Populations in the Massive Globular Cluster M80","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Globular cluster; Physics; Astrophysics; Cluster (spacecraft); Hubble space telescope; Stars; Mass segregation; Distribution (mathematics); Star cluster; Mathematics; Mathematical analysis","score_opus":0.0159869117521815,"score_gpt":0.2498699730604561,"score_spread":0.2338830613082746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797165970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994887,0.000022693084,0.00017566362,0.000006638472,3.9511104e-7,9.995123e-7,0.00006499053,0.000013276242,0.00022663812],"genre_scores_gemma":[0.9994797,0.000011370472,0.00023849016,0.0000022467088,0.0000010754505,0.00000170006,0.0001682879,0.000005754959,0.00009137551],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994874,0.000006552924,0.0000020026519,0.00001839765,0.00001312916,0.000011119167],"domain_scores_gemma":[0.99979013,0.00004643783,0.000051570456,0.000024997633,0.000033668384,0.00005327384],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001787772,0.00019934596,0.00019528254,0.0007063864,0.0002596581,0.00029674455,0.00042035017,0.00021462851,0.0006409401],"category_scores_gemma":[0.0005695655,0.00013725513,0.00024153267,0.0003286739,0.00024566584,0.00016764298,0.0004535135,0.00010465409,0.0001601625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028049867,0.00008006136,0.83806044,0.000052529966,0.00017487626,0.00058171304,0.00039683192,0.10291389,0.04533259,0.0023605877,0.00061971234,0.009146282],"study_design_scores_gemma":[0.00002466241,0.000083506435,0.7830765,0.000009566946,0.000045627068,0.00022035284,0.0001648292,0.21100819,0.0034654455,0.0009745324,0.0008996485,0.000027105374],"about_ca_topic_score_codex":0.0073540015,"about_ca_topic_score_gemma":0.0068692635,"teacher_disagreement_score":0.0073540015,"about_ca_system_score_codex":0.00057197333,"about_ca_system_score_gemma":0.000188631,"threshold_uncertainty_score":0.01462239},"labels":[],"label_agreement":null},{"id":"W2797217417","doi":"10.3847/1538-4357/aac2d2","title":"Polycrystalline Crusts in Accreting Neutron Stars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Neutron star; Crust; Stars; Dense matter; Pulsar; Accretion (finance); s-process; Crystallite","score_opus":0.012896078415487143,"score_gpt":0.3211276970722264,"score_spread":0.30823161865673926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797217417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956553,0.00025801425,0.0026927143,0.0000200905,0.0000037937896,0.0000056910267,0.00009424623,0.000031679698,0.0012384801],"genre_scores_gemma":[0.9989354,0.00006494867,0.0007507399,0.000004462543,0.000001195619,0.0000021720405,0.00006802421,0.000007486243,0.00016552687],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992394,0.0000064338933,0.000006850098,0.000025745638,0.000022235226,0.000014762328],"domain_scores_gemma":[0.99968505,0.0000654292,0.00013734766,0.00003424946,0.000035258894,0.000042605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011717526,0.00013268429,0.00019394298,0.00059441477,0.0002959859,0.0009871691,0.00021530365,0.00026204664,0.001676418],"category_scores_gemma":[0.0005113632,0.00021454768,0.00014905934,0.00032332703,0.0006209328,0.0005052976,0.00037574797,0.00021718466,0.00015152288],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006043044,0.00014765654,0.12658323,0.00026145918,0.00015787664,0.0015911784,0.00030679585,0.08711099,0.7467729,0.019437548,0.00028590916,0.016740233],"study_design_scores_gemma":[0.00019046165,0.00036069305,0.36353508,0.00009025517,0.0001014324,0.003085717,0.00096818956,0.31043297,0.28078827,0.03212873,0.008231867,0.00008637913],"about_ca_topic_score_codex":0.0008423453,"about_ca_topic_score_gemma":0.0006285761,"teacher_disagreement_score":0.001676418,"about_ca_system_score_codex":0.00030719052,"about_ca_system_score_gemma":0.00014975056,"threshold_uncertainty_score":0.0056081414},"labels":[],"label_agreement":null},{"id":"W2797237446","doi":"10.3847/1538-4357/aabfc4","title":"Revisiting the Stellar Mass–Angular Momentum–Morphology Relation: Extension to Higher Bulge Fraction and the Effect of Bulge Type","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; Instituto de Astrofísica de Andalucía; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Australian Research Council; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ohio State University; Carnegie Institution of Washington; Leibniz-Gemeinschaft; University of Notre Dame; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Bulge; Physics; Astrophysics; Galaxy; Angular momentum; BETA (programming language); Dark matter; Stellar mass; Star formation; Classical mechanics","score_opus":0.005881415288330145,"score_gpt":0.22212187618806603,"score_spread":0.2162404608997359,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797237446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99837625,0.00027922925,0.00041001046,0.000077432305,0.000004117914,0.000002720042,0.00013794076,0.000019240302,0.0006930338],"genre_scores_gemma":[0.99970716,0.000027090922,0.000086459935,0.00001749854,0.00000419247,8.708836e-7,0.00008110092,0.000005650847,0.00007000791],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994961,0.00020455076,0.000030156569,0.00012912696,0.0000741214,0.00006592167],"domain_scores_gemma":[0.9931443,0.0042235884,0.0011125477,0.00071536587,0.00031732605,0.00048697233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017743676,0.00035488824,0.00032768582,0.001283926,0.00031799136,0.0009635033,0.00061375555,0.00041515543,0.0023853034],"category_scores_gemma":[0.0055542663,0.00020337889,0.0006753255,0.0010230991,0.00078037044,0.00069895905,0.00071225356,0.0006089946,0.00035100465],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007938746,0.000015833308,0.99606687,0.000006370909,0.000057290796,0.000047322705,0.00007136322,0.00025153867,0.0012014301,0.000041577594,0.000053065876,0.0021079744],"study_design_scores_gemma":[0.0000012467608,0.000039958777,0.998733,0.000003320947,0.000023400624,0.00004349995,0.00009229962,0.00069468317,0.00022278335,0.00003444636,0.00010943303,0.0000020428645],"about_ca_topic_score_codex":0.013037053,"about_ca_topic_score_gemma":0.010203962,"teacher_disagreement_score":0.013037053,"about_ca_system_score_codex":0.0002527936,"about_ca_system_score_gemma":0.00026465562,"threshold_uncertainty_score":0.025922358},"labels":[],"label_agreement":null},{"id":"W2797239254","doi":"10.3847/1538-4357/aabe8c","title":"The Dust and [C ii] Morphologies of Redshift ∼4.5 Sub-millimeter Galaxies at ∼200 pc Resolution: The Absence of Large Clumps in the Interstellar Medium at High-redshift","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"National Institutes of Natural Sciences; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Science and Technology Facilities Council; National Astronomical Observatory of Japan; European Commission; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Redshift; Substructure; Galaxy; Millimeter; Star formation; Interstellar medium; Rest frame; Emission spectrum; Spectral line; Astronomy","score_opus":0.009281019774845783,"score_gpt":0.2202368790703396,"score_spread":0.21095585929549382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797239254","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993967,0.00003410909,0.00017503093,0.0000072738953,6.7015407e-7,9.327409e-7,0.000083808656,0.000026911965,0.00027448396],"genre_scores_gemma":[0.99940765,0.000013858146,0.00029032276,0.000006284615,0.0000025609434,0.0000010249543,0.000203657,0.0000035376254,0.00007124986],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992335,0.0000056800704,0.0000038119426,0.000019549698,0.00002242301,0.000025200052],"domain_scores_gemma":[0.99969125,0.000038420196,0.00010419151,0.000050151168,0.000041953812,0.00007410223],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014411536,0.00016719633,0.00017777007,0.0007439233,0.00018620801,0.000508431,0.00023506006,0.00017541274,0.000806949],"category_scores_gemma":[0.00032300293,0.0001941976,0.00021087482,0.00040820419,0.00020305355,0.00016588402,0.00029491467,0.00016739381,0.00021745899],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014324424,0.00003657411,0.86732036,0.000023611949,0.000087533306,0.00023458594,0.00032531627,0.0008969644,0.1218728,0.000137491,0.00027046757,0.008651089],"study_design_scores_gemma":[0.0000018319305,0.000008194202,0.99782616,0.0000013468498,0.000008314641,0.000065159475,0.00004114737,0.00051308505,0.0013575046,0.00001691981,0.00015896777,0.0000013463567],"about_ca_topic_score_codex":0.0034598836,"about_ca_topic_score_gemma":0.0046694623,"teacher_disagreement_score":0.0034598836,"about_ca_system_score_codex":0.00026152574,"about_ca_system_score_gemma":0.000060922397,"threshold_uncertainty_score":0.006879449},"labels":[],"label_agreement":null},{"id":"W2797405913","doi":"10.3847/1538-4357/aac5f3","title":"ALMA Resolves C i Emission from the β Pictoris Debris Disk","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Debris disk; Planet; Debris; Accretion (finance); Protoplanet; Planetary system; Accretion disc; Mass ratio","score_opus":0.01145571821845093,"score_gpt":0.2452032669838101,"score_spread":0.23374754876535916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797405913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9899328,0.0004016456,0.002065773,0.00018546905,0.000023165472,0.000020567872,0.00068460696,0.00031682523,0.0063693547],"genre_scores_gemma":[0.99652654,0.000067720786,0.0025196555,0.00007954575,0.000034662033,0.0000130342105,0.0002662134,0.00002086754,0.00047178523],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999056,0.0000102183,0.0000026774246,0.000036093286,0.000015905973,0.000029579847],"domain_scores_gemma":[0.9997677,0.000059516708,0.000052994557,0.000033187192,0.000030429803,0.000056209414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020176513,0.00021864612,0.000198671,0.001589296,0.00047093662,0.0006467853,0.00028108165,0.0003969877,0.0023576678],"category_scores_gemma":[0.00033779902,0.00020101338,0.0002033246,0.00058604043,0.00018365547,0.0003009599,0.0002821683,0.00029438428,0.00042701737],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011684361,0.00023244628,0.22899336,0.00010875407,0.00016070143,0.0013704455,0.00048566423,0.0011407882,0.7278476,0.0007652632,0.003580179,0.0341464],"study_design_scores_gemma":[0.00008238575,0.00019212982,0.9336928,0.00003899522,0.00012691549,0.0010260575,0.000320173,0.008790756,0.048491243,0.000643065,0.006560636,0.000034801815],"about_ca_topic_score_codex":0.0007900568,"about_ca_topic_score_gemma":0.0017028376,"teacher_disagreement_score":0.0023576678,"about_ca_system_score_codex":0.00027017528,"about_ca_system_score_gemma":0.000077072946,"threshold_uncertainty_score":0.007887185},"labels":[],"label_agreement":null},{"id":"W2797460355","doi":"10.3847/1538-4357/aad005","title":"Highest Frequency Detection of FRB 121102 at 4–8 GHz Using the Breakthrough Listen Digital Backend at the Green Bank Telescope","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":324,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University","funders":"Secretário de Ciência, Tecnologia e Ensino Superior, Governo do Estado de Parana; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Breakthrough Prize Foundation; Max-Planck-Gesellschaft; National Science Foundation","keywords":"Physics; Fast radio burst; Astrophysics; Radio telescope; Polarization (electrochemistry); Position angle; Telescope; Scintillation; Green Bank Telescope; Linear polarization; Radio spectrum; Optics; Galaxy; Astronomy; Detector","score_opus":0.018015223927909524,"score_gpt":0.30077973184446977,"score_spread":0.28276450791656027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797460355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99554247,0.0001782887,0.001188155,0.00004689111,0.000013231619,0.000007028292,0.00046639217,0.00012922454,0.0024285456],"genre_scores_gemma":[0.9968593,0.000054128555,0.0010524524,0.000027895378,0.000018711627,0.000006485062,0.00093758974,0.000016935704,0.0010266415],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99983287,0.000012499345,0.0000057881134,0.000041088028,0.00006474838,0.000042996853],"domain_scores_gemma":[0.9996636,0.000054474258,0.000090911686,0.000040885727,0.000053035546,0.00009709836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022698665,0.00020506515,0.00025006273,0.0008605533,0.0002843135,0.00043624084,0.0003383197,0.00033600442,0.0025741153],"category_scores_gemma":[0.00038428383,0.00021204949,0.00012364922,0.0003777119,0.00020106608,0.00017479833,0.00035933303,0.00037365363,0.00081890804],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011749632,0.00014814569,0.28918833,0.00009839938,0.00009575693,0.0016265067,0.00061233423,0.00089345884,0.66768456,0.00028609243,0.0029266456,0.035264827],"study_design_scores_gemma":[0.00004390871,0.00037689382,0.96155745,0.000026830488,0.000045150133,0.0011804498,0.00019559836,0.0017237068,0.02860856,0.000075319185,0.006135194,0.00003111679],"about_ca_topic_score_codex":0.0029856593,"about_ca_topic_score_gemma":0.0062177703,"teacher_disagreement_score":0.0029856593,"about_ca_system_score_codex":0.00036176006,"about_ca_system_score_gemma":0.00011365095,"threshold_uncertainty_score":0.008611262},"labels":[],"label_agreement":null},{"id":"W2797518049","doi":"10.3847/1538-4357/aabe8d","title":"The Frequency of Intrinsic X-Ray Weakness among Broad Absorption Line Quasars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Quasar; Astrophysics; Physics; Population; OVV quasar; Spectral line; Astronomy; Galaxy; Medicine","score_opus":0.007518589873208372,"score_gpt":0.2202702542577751,"score_spread":0.21275166438456675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797518049","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994748,0.00006761894,0.00008879209,0.000007318797,7.4716894e-7,0.0000010378598,0.000052527957,0.0000059114072,0.00030136135],"genre_scores_gemma":[0.99983335,0.000013045848,0.000034598288,0.000004466303,0.000002592052,6.232124e-7,0.00006723044,0.0000010472957,0.000042998556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997211,0.000035888123,0.000021955257,0.000068579604,0.00007690438,0.00007563444],"domain_scores_gemma":[0.9981888,0.0003460376,0.00067461474,0.00019544142,0.00028136533,0.0003137382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043932104,0.00013919565,0.00021631748,0.0015572201,0.00030715566,0.00066579366,0.00031036808,0.00019613662,0.0014027181],"category_scores_gemma":[0.0013121576,0.00014844177,0.00012215711,0.00055032695,0.00048922416,0.00038706025,0.0006129625,0.00024885853,0.0001796898],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000027273727,0.000011324958,0.9941717,0.0000043459627,0.000016271495,0.000043080418,0.000075722215,0.000032316926,0.003653788,0.000037109676,0.000033684755,0.0018934725],"study_design_scores_gemma":[8.2599547e-7,0.000014843134,0.9992957,9.678698e-7,0.000005229247,0.00012866448,0.000052897347,0.00008789994,0.0003299747,0.000016456384,0.00006511544,0.0000013341887],"about_ca_topic_score_codex":0.0018679703,"about_ca_topic_score_gemma":0.0024155648,"teacher_disagreement_score":0.0018679703,"about_ca_system_score_codex":0.00016038974,"about_ca_system_score_gemma":0.00007109339,"threshold_uncertainty_score":0.004692495},"labels":[],"label_agreement":null},{"id":"W2797616721","doi":"10.3847/1538-4357/ab0af0","title":"Weak-lensing Mass Calibration of ACTPol Sunyaev–Zel’dovich Clusters with the Hyper Suprime-Cam Survey","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Economic and Social Research Council","keywords":"Cosmic microwave background; Cosmology; South Pole Telescope; Galaxy cluster; Planck; Mass distribution; Hydrostatic equilibrium; Telescope; Cluster (spacecraft); Subaru Telescope","score_opus":0.00812817518702183,"score_gpt":0.20190034701297888,"score_spread":0.19377217182595705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2797616721","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978338,0.00007648897,0.00033563114,0.00003059096,0.0000060788066,0.0000052724513,0.00046701892,0.000017658573,0.0012274206],"genre_scores_gemma":[0.9986243,0.000024275963,0.00030593,0.0000074505697,0.0000075001735,0.000004578577,0.0009010119,0.0000083274845,0.00011655096],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996138,0.00009419058,0.000020715348,0.00011303365,0.000089295805,0.000069029964],"domain_scores_gemma":[0.99841,0.00019780715,0.0004658354,0.00034581684,0.0002407778,0.00033969848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009895369,0.00034824404,0.00028668923,0.0011034901,0.00043206438,0.0006574299,0.00053645,0.00016892522,0.0007580161],"category_scores_gemma":[0.0016904556,0.00021595787,0.00023253667,0.0006453912,0.00031046307,0.0001933606,0.00095826766,0.00026765093,0.00021681264],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016911373,0.0000174638,0.98900336,0.000012621881,0.00006873837,0.000045322115,0.00013761244,0.00195437,0.0037259525,0.00034396633,0.0005965724,0.0039248094],"study_design_scores_gemma":[0.000008085875,0.000012444191,0.9956879,0.0000052630594,0.00001183931,0.000013676828,0.000043722375,0.002917772,0.00084955705,0.000034619523,0.00041087478,0.000004281156],"about_ca_topic_score_codex":0.026573256,"about_ca_topic_score_gemma":0.03732329,"teacher_disagreement_score":0.026573256,"about_ca_system_score_codex":0.00075767626,"about_ca_system_score_gemma":0.0003254234,"threshold_uncertainty_score":0.052837133},"labels":[],"label_agreement":null},{"id":"W2798013443","doi":"10.3847/1538-4357/aabe92","title":"Growth of Beam–Plasma Instabilities in the Presence of Background Inhomogeneity","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Instability; Plasma; Physics; Beam (structure); Two-stream instability; Saturation (graph theory); Growth rate; Atomic physics; Homogeneous; Astrophysics; Optics; Mechanics; Nuclear physics; Geometry; Statistical physics","score_opus":0.015177988397084084,"score_gpt":0.23749593275196995,"score_spread":0.22231794435488586,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798013443","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960556,0.00007277928,0.0020176433,0.00006744001,0.0000076236865,0.0000074910754,0.000078071615,0.00006952759,0.0016237099],"genre_scores_gemma":[0.99923384,0.000026663298,0.00047369403,0.0000075541325,0.0000024692451,0.000004829497,0.000047546022,0.000015472617,0.00018787807],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99988604,0.000017056294,0.000005028804,0.00001986006,0.000023563158,0.00004846119],"domain_scores_gemma":[0.9993662,0.00032586642,0.00010341322,0.00004284158,0.00007437636,0.000087342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022290359,0.00032449586,0.00027140783,0.00034806295,0.0003240825,0.0008049127,0.00041821302,0.00041872644,0.00136901],"category_scores_gemma":[0.001602616,0.00017510461,0.00030043555,0.00021947302,0.0005108446,0.0005352887,0.0006009363,0.00054271024,0.00012590867],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006221273,0.00023180089,0.034105774,0.00018161295,0.00016275643,0.001070017,0.00035898018,0.6759254,0.2717547,0.006804591,0.00095454784,0.007827722],"study_design_scores_gemma":[0.000040908573,0.00010799405,0.009353472,0.000007027189,0.000020286354,0.000069433496,0.000083409555,0.9546007,0.03469281,0.0006964887,0.00030779518,0.000019608764],"about_ca_topic_score_codex":0.0040089297,"about_ca_topic_score_gemma":0.0013889372,"teacher_disagreement_score":0.0040089297,"about_ca_system_score_codex":0.0004998315,"about_ca_system_score_gemma":0.00033649552,"threshold_uncertainty_score":0.007971168},"labels":[],"label_agreement":null},{"id":"W2798316210","doi":"10.3847/1538-4357/aac088","title":"Extended Millimeter Emission in the HD 141569 Circumstellar Disk Detected with ALMA","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Spectral index; Millimeter; Circumstellar disk; Visibility; Emission spectrum; Debris disk; Circumstellar dust","score_opus":0.009606495404542963,"score_gpt":0.23464522998796222,"score_spread":0.22503873458341925,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798316210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904376,0.000043670796,0.00014853162,0.000008809095,0.000002667838,0.0000014701579,0.00011786539,0.000010662543,0.0006225453],"genre_scores_gemma":[0.99959177,0.000012554516,0.00013651024,0.0000046374516,0.000002805922,0.0000014425435,0.00016667033,0.0000014623747,0.00008215941],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998853,0.00000995355,0.000007634549,0.000042550633,0.000032631735,0.00002181474],"domain_scores_gemma":[0.9998229,0.000024003342,0.00005342476,0.000026016945,0.000024221361,0.00004950227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016498503,0.00015730422,0.0002573706,0.0005036072,0.00040394624,0.0004952618,0.00024551153,0.00018859163,0.00088239065],"category_scores_gemma":[0.0003500753,0.00014648156,0.00020644059,0.00035036044,0.00017522802,0.00022530225,0.00043530285,0.00018193154,0.00022762058],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040921607,0.00009249986,0.79519653,0.000048923208,0.00010327828,0.0007089353,0.00039235188,0.0014129116,0.19212736,0.00042835,0.00035269602,0.00872693],"study_design_scores_gemma":[0.0000097742095,0.000041068473,0.99390334,0.0000035711869,0.000017312146,0.00022015594,0.00010414068,0.0014469249,0.0035559281,0.0000653942,0.00062672404,0.0000056296144],"about_ca_topic_score_codex":0.0020227365,"about_ca_topic_score_gemma":0.0027970076,"teacher_disagreement_score":0.0020227365,"about_ca_system_score_codex":0.00033248446,"about_ca_system_score_gemma":0.00008239338,"threshold_uncertainty_score":0.0040219426},"labels":[],"label_agreement":null},{"id":"W2798441981","doi":"10.3847/1538-4357/aad9f9","title":"The Origin of the 300 km s<sup>−1</sup> Stream near Segue 1","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Dwarf galaxy; Metallicity; Galaxy; Luminosity; Stars; Local Group; Galactic halo","score_opus":0.01066321477848078,"score_gpt":0.23100237457109188,"score_spread":0.2203391597926111,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798441981","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980221,0.000044042998,0.00020498772,0.000033769837,0.0000056853987,0.0000041789463,0.0001463311,0.00003414426,0.0015048146],"genre_scores_gemma":[0.99811494,0.000040925097,0.00046040365,0.000014347974,0.000009907029,0.0000038665507,0.00051802135,0.000009012465,0.00082858204],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993646,0.0000044186713,0.000003067486,0.000017202534,0.000018275015,0.000020577467],"domain_scores_gemma":[0.9996449,0.000031486154,0.00011352158,0.00002801695,0.000047678714,0.00013443353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000095666095,0.00014198844,0.00017375476,0.0008174377,0.00037603732,0.00082897797,0.00024720575,0.00029843155,0.002979881],"category_scores_gemma":[0.00041461125,0.00009762441,0.00010500107,0.00053367426,0.00024908336,0.00033893454,0.00052957766,0.00016759137,0.00083126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023383283,0.00004460752,0.9399173,0.000035131183,0.000018421955,0.0011941083,0.00090947247,0.00034575394,0.033623803,0.0007764595,0.0009291773,0.02197189],"study_design_scores_gemma":[0.000007702928,0.00012220415,0.9843694,0.000012515399,0.000013727529,0.0008103175,0.00091664394,0.00090356346,0.005316793,0.00035868335,0.0071597006,0.0000087606095],"about_ca_topic_score_codex":0.0020577682,"about_ca_topic_score_gemma":0.0035301785,"teacher_disagreement_score":0.002979881,"about_ca_system_score_codex":0.00026029637,"about_ca_system_score_gemma":0.00014864233,"threshold_uncertainty_score":0.009968698},"labels":[],"label_agreement":null},{"id":"W2798512692","doi":"10.3847/1538-4357/aadfee","title":"The Missing Satellites of the Magellanic Clouds? Gaia Proper Motions of the Recently Discovered Ultra-faint Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Milky Way; Galaxy; Large Magellanic Cloud; Dwarf galaxy; Local Group; Proper motion; Stars; Satellite galaxy","score_opus":0.012709722474699313,"score_gpt":0.2555916079244614,"score_spread":0.24288188544976208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798512692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987589,0.00008131319,0.00033664927,0.00003872584,0.0000022013244,0.0000013489602,0.00023112295,0.00003908511,0.0005106354],"genre_scores_gemma":[0.999438,0.000012043345,0.0002750813,0.0000051240677,0.0000013683211,6.521818e-7,0.00019964112,0.0000044054295,0.00006377057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999144,0.000012950634,0.000004824829,0.000025991152,0.000018766952,0.000023196048],"domain_scores_gemma":[0.99960977,0.00005661605,0.00012837577,0.00008683914,0.000035790308,0.00008268495],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018837184,0.00013316504,0.00023181524,0.0005828778,0.0002695521,0.000541646,0.0003506558,0.0002199991,0.00061042764],"category_scores_gemma":[0.00063340756,0.00012348333,0.000251804,0.00056638045,0.00021372325,0.00033389128,0.00031508645,0.00022399996,0.0001831342],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014329144,0.000021677388,0.97310084,0.000024269422,0.000064466694,0.00021819827,0.00020342584,0.003955941,0.0135942055,0.0012036621,0.00046466824,0.007005229],"study_design_scores_gemma":[0.000008556776,0.000025555879,0.9839108,0.0000053174335,0.000019538635,0.00015605862,0.00011502455,0.011647808,0.002528462,0.00025672902,0.0013188473,0.0000072281505],"about_ca_topic_score_codex":0.008822781,"about_ca_topic_score_gemma":0.0099564735,"teacher_disagreement_score":0.008822781,"about_ca_system_score_codex":0.0006948814,"about_ca_system_score_gemma":0.0001838659,"threshold_uncertainty_score":0.017542839},"labels":[],"label_agreement":null},{"id":"W2798628623","doi":"10.3847/1538-4357/aac018","title":"The Circumstellar Disk and Asymmetric Outflow of the EX Lup Outburst System","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Outflow; Radiative transfer; RADIUS; Circumstellar disk; Accretion (finance); Isotopologue; Population; Submillimeter Array; Protostar","score_opus":0.006805167579643131,"score_gpt":0.21411289122847205,"score_spread":0.2073077236488289,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798628623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951327,0.000023657412,0.00004682372,0.0000053745516,7.900701e-7,0.0000012695215,0.00003778421,0.0000044676676,0.00036645719],"genre_scores_gemma":[0.9998343,0.000007750765,0.000039413764,0.000004102534,0.0000016162015,6.7923094e-7,0.000059036476,7.909745e-7,0.000052186977],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999491,0.0000060786883,0.0000033007645,0.0000144537935,0.000008269917,0.00001885763],"domain_scores_gemma":[0.99985886,0.000013593259,0.000053928143,0.000013334817,0.00001370612,0.000046589492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009652802,0.00017765346,0.00014547267,0.00034648212,0.00043520576,0.00043127165,0.00018411748,0.00016896438,0.00076116406],"category_scores_gemma":[0.0002513279,0.00008514539,0.00007453952,0.00017536207,0.00022209171,0.00019379768,0.00040589905,0.00012014998,0.000112496295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003230728,0.00007692541,0.9512657,0.000019448047,0.000022631586,0.0022117111,0.0005155254,0.00027522576,0.03791785,0.00019286775,0.00019748895,0.0069815116],"study_design_scores_gemma":[0.000006555025,0.000047528254,0.99743634,0.0000040263317,0.000007024599,0.0006660151,0.00022740272,0.0004678214,0.00066938484,0.000054137272,0.00041142755,0.000002470588],"about_ca_topic_score_codex":0.0023057943,"about_ca_topic_score_gemma":0.0027469466,"teacher_disagreement_score":0.0023057943,"about_ca_system_score_codex":0.0002230975,"about_ca_system_score_gemma":0.00007051321,"threshold_uncertainty_score":0.0045847893},"labels":[],"label_agreement":null},{"id":"W2798697049","doi":"10.3847/1538-4357/aac326","title":"Cloud-scale Molecular Gas Properties in 15 Nearby Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":237,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galaxy; Virial theorem; Milky Way; Line (geometry); Spiral galaxy; Interstellar medium; Measure (data warehouse); Spectral line; Luminous infrared galaxy","score_opus":0.00988617145545999,"score_gpt":0.22218378183288523,"score_spread":0.21229761037742523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798697049","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997967,0.000023499206,0.000028083485,0.0000018215401,3.068878e-7,0.0000010480444,0.00008812157,0.0000020072132,0.000058428115],"genre_scores_gemma":[0.9995308,0.000013735742,0.00006808527,0.0000031516977,0.0000017048195,0.0000014096165,0.0003293197,0.0000011223854,0.000050776984],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997981,0.000020439169,0.000013862927,0.00008101399,0.000040016657,0.000046608926],"domain_scores_gemma":[0.9993736,0.00007333024,0.00020376196,0.000071343435,0.000060890612,0.00021712037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022999366,0.00023587728,0.00026809584,0.0014231353,0.00038195404,0.0005715461,0.00029771368,0.00028108244,0.00060354423],"category_scores_gemma":[0.00066684117,0.0001797174,0.00022753401,0.0010462676,0.00038263557,0.00034442014,0.0005874702,0.00014719016,0.00023369424],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046951372,0.000023315697,0.9950723,0.000004431288,0.00003858757,0.000046440273,0.00019734829,0.0001341374,0.0030897756,0.000029562083,0.000026582555,0.0012905694],"study_design_scores_gemma":[0.0000023014898,0.00003081454,0.99899226,0.0000012010642,0.000007736633,0.00006071693,0.000109613015,0.00032755814,0.00033601932,0.000017141274,0.000112689326,0.0000020383925],"about_ca_topic_score_codex":0.010815041,"about_ca_topic_score_gemma":0.013957817,"teacher_disagreement_score":0.010815041,"about_ca_system_score_codex":0.00038761095,"about_ca_system_score_gemma":0.00011276737,"threshold_uncertainty_score":0.021504223},"labels":[],"label_agreement":null},{"id":"W2798726971","doi":"10.3847/1538-4357/aabf94","title":"Homogeneous Analysis of the Dust Morphology of Transition Disks Observed with ALMA: Investigating Dust Trapping and the Origin of the Cavities","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Physics; Millimeter; Photoevaporation; Astrophysics; Submillimeter Array; Planet; Context (archaeology); Star formation; Stars","score_opus":0.022953710280342578,"score_gpt":0.2328600266717745,"score_spread":0.20990631639143192,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798726971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990238,0.000051304727,0.00039466223,0.0000042164925,9.993541e-7,0.0000035011299,0.00013887447,0.000013878649,0.00036885877],"genre_scores_gemma":[0.9995615,0.000008252014,0.00027286317,0.0000024216424,0.0000018739324,0.0000017148385,0.00009208179,0.00000243886,0.000056880006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999323,0.0000066820016,0.000004487727,0.000022147984,0.000015901787,0.0000185044],"domain_scores_gemma":[0.99968886,0.00006615937,0.000100668796,0.000035732366,0.000056250563,0.000052324896],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008391798,0.000116270385,0.00014929817,0.00093665975,0.00017340768,0.00040797758,0.0001873946,0.00014606606,0.0008613249],"category_scores_gemma":[0.0002596212,0.00007899908,0.00017657097,0.00047492696,0.0001407778,0.00023490614,0.00025206173,0.00011718186,0.00015171255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028508026,0.000045114204,0.76521593,0.000037277492,0.00006424104,0.00036672183,0.00024955175,0.00051208923,0.22243093,0.00012319107,0.0001423549,0.010527369],"study_design_scores_gemma":[0.0000021699425,0.000029706178,0.99462885,0.0000011606483,0.000010619839,0.00012041551,0.000098186785,0.0010111926,0.0039190548,0.000027416403,0.00014896994,0.0000022977529],"about_ca_topic_score_codex":0.0012521496,"about_ca_topic_score_gemma":0.0013941593,"teacher_disagreement_score":0.0012521496,"about_ca_system_score_codex":0.00015725667,"about_ca_system_score_gemma":0.000043854317,"threshold_uncertainty_score":0.0028814077},"labels":[],"label_agreement":null},{"id":"W2798922034","doi":"10.3847/1538-4357/aacd0e","title":"A Deeper Look at the New Milky Way Satellites: Sagittarius II, Reticulum II, Phoenix II, and Tucana III<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Globular cluster; Milky Way; Dwarf galaxy; Sagittarius; Dwarf spheroidal galaxy; Star cluster; Galaxy","score_opus":0.008210893657248957,"score_gpt":0.21203596852388698,"score_spread":0.20382507486663803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798922034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99567187,0.00018633163,0.00019419896,0.000072717325,0.0000055109554,0.0000031922045,0.0006565304,0.000024702345,0.003184978],"genre_scores_gemma":[0.99630475,0.00007900465,0.00062124105,0.00006198479,0.000012299885,0.0000024223816,0.0017274272,0.000012451176,0.0011783952],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999685,0.0000016173715,0.0000015193478,0.00000899503,0.000007853734,0.000011381827],"domain_scores_gemma":[0.9998473,0.000021193737,0.000039281553,0.000010789846,0.000029540544,0.00005185516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008925064,0.00014171306,0.00011962959,0.0011552381,0.00033002687,0.00050421746,0.00017594628,0.00021249715,0.0032047462],"category_scores_gemma":[0.0001367664,0.00007417661,0.0001429298,0.00079483225,0.00020587545,0.00034219114,0.00035822892,0.00026108575,0.00024204585],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016293753,0.0000411501,0.8915054,0.00005437903,0.000063426975,0.0008765984,0.0012440025,0.00049344177,0.07609374,0.0005928715,0.0016936774,0.027178371],"study_design_scores_gemma":[0.000003503791,0.000019523635,0.98837763,0.000007644377,0.000017092547,0.00027453306,0.00082765345,0.00031973628,0.0031192654,0.0000728879,0.00695434,0.0000061701285],"about_ca_topic_score_codex":0.01534145,"about_ca_topic_score_gemma":0.037257385,"teacher_disagreement_score":0.01534145,"about_ca_system_score_codex":0.00040642123,"about_ca_system_score_gemma":0.00014495938,"threshold_uncertainty_score":0.030504346},"labels":[],"label_agreement":null},{"id":"W2798933185","doi":"10.3847/1538-4357/aabfbe","title":"A Universal Spin–Mass Relation for Brown Dwarfs and Planets","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Brown dwarf; Physics; Astrophysics; Planet; Angular momentum; Planetary mass; Astronomy; Solar System; Solar mass; Rotation period; Exoplanet; Stars; Classical mechanics","score_opus":0.011273130730540513,"score_gpt":0.22773021190455764,"score_spread":0.21645708117401713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798933185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99669194,0.00015598384,0.0011298942,0.00001681324,0.0000034471807,0.000003428218,0.00016682406,0.000040242343,0.0017913575],"genre_scores_gemma":[0.9994956,0.000017726685,0.00023338532,0.0000053673166,0.0000036936867,0.0000012224615,0.000102622136,0.000003012538,0.00013732766],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982363,0.000020754502,0.000015361007,0.000070880655,0.000033025466,0.000036385256],"domain_scores_gemma":[0.99808383,0.0005257375,0.00067882246,0.00026741708,0.00022719342,0.0002171522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029145312,0.00015456132,0.00018557896,0.000999706,0.00029555472,0.00058110803,0.00014303083,0.00022364632,0.0018696738],"category_scores_gemma":[0.002583928,0.0001236451,0.0001449432,0.0004936845,0.00043005275,0.00040277618,0.0003789033,0.00016757683,0.00052597927],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010111929,0.00001540056,0.9794867,0.000012454377,0.000024895111,0.00008965167,0.00021852557,0.00023304606,0.011271537,0.0003841446,0.00009805753,0.008064451],"study_design_scores_gemma":[0.0000029601842,0.00005092286,0.9961641,0.0000029285668,0.000007679686,0.00040760904,0.00010071732,0.0007248169,0.0017341211,0.00043492313,0.0003659707,0.000003329298],"about_ca_topic_score_codex":0.0010997457,"about_ca_topic_score_gemma":0.0011919945,"teacher_disagreement_score":0.0018696738,"about_ca_system_score_codex":0.00019163676,"about_ca_system_score_gemma":0.00010165193,"threshold_uncertainty_score":0.006254673},"labels":[],"label_agreement":null},{"id":"W2798952077","doi":"10.3847/1538-4357/ab1eb0","title":"Relative Alignment between the Magnetic Field and Molecular Gas Structure in the Vela C Giant Molecular Cloud Using Low- and High-density Tracers","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Vela; Molecular cloud; Magnetic field; Radiative transfer; Polarimeter; Orientation (vector space); Perpendicular; Polarization (electrochemistry)","score_opus":0.004910617786583943,"score_gpt":0.21281485459488092,"score_spread":0.20790423680829698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798952077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939823,0.000024555078,0.000077419514,0.000009530916,5.3733254e-7,0.0000015799892,0.00009576916,0.000008685459,0.0003835661],"genre_scores_gemma":[0.9996544,0.000013008854,0.00011844974,0.0000043891505,0.0000013824333,0.000001454645,0.00016575062,0.0000033329623,0.00003774467],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999105,0.000007942274,0.0000036608033,0.000026007714,0.000020351037,0.000031498457],"domain_scores_gemma":[0.9996214,0.00006120114,0.00012078127,0.000029830697,0.000059140766,0.00010761785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016478113,0.00010871742,0.00016705258,0.0010099501,0.00036622278,0.000608692,0.00030433433,0.00020851515,0.00047847079],"category_scores_gemma":[0.00074911834,0.00013789347,0.00014311691,0.00060950854,0.00030028494,0.00020808,0.0005019002,0.00019814924,0.000075646865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002894719,0.000048565966,0.8893532,0.000033463362,0.000094153416,0.00023960124,0.00034379965,0.0058199433,0.097831905,0.00038527025,0.00014051754,0.0054201395],"study_design_scores_gemma":[0.000009180192,0.000016031134,0.99262094,0.0000051223537,0.000010007919,0.000045877463,0.0000957172,0.005244035,0.0017883966,0.000044542274,0.00011334971,0.000006745676],"about_ca_topic_score_codex":0.024788361,"about_ca_topic_score_gemma":0.024023436,"teacher_disagreement_score":0.024788361,"about_ca_system_score_codex":0.0007115307,"about_ca_system_score_gemma":0.00028009372,"threshold_uncertainty_score":0.049288154},"labels":[],"label_agreement":null},{"id":"W2798993641","doi":"10.3847/1538-4357/aac103","title":"MESAS: Measuring the Emission of Stellar Atmospheres at Submillimeter/millimeter Wavelengths","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Millimeter; Stars; Physics; Astrophysics; Astronomy; Sirius; Wavelength; Atmosphere (unit); Planet; Stellar atmosphere; Optics","score_opus":0.015128958343479534,"score_gpt":0.23471428780011774,"score_spread":0.21958532945663822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2798993641","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97597605,0.00015931585,0.005455715,0.000087523294,0.000016225516,0.000031741063,0.003991734,0.0010791128,0.013202561],"genre_scores_gemma":[0.9831738,0.00009979804,0.01304799,0.000053667936,0.000022847733,0.000017033713,0.0018169774,0.00004568712,0.0017221344],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991345,0.000012305894,0.00000362905,0.000035957626,0.00002539103,0.00000931918],"domain_scores_gemma":[0.99980897,0.000031707852,0.00005438474,0.000041800515,0.000024618103,0.000038525373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025084,0.00019544497,0.00009543047,0.00047696623,0.00019703692,0.0003427501,0.00027270656,0.00015074611,0.0018578521],"category_scores_gemma":[0.00022572475,0.00016241196,0.00020741961,0.00025403866,0.000090760324,0.00026117836,0.00027477043,0.0002349879,0.00055007945],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007506077,0.00016591772,0.6683957,0.000105298284,0.00024118814,0.00017552568,0.00034926797,0.006308743,0.2742671,0.0022221191,0.0057960562,0.0412225],"study_design_scores_gemma":[0.000051435993,0.00017600715,0.9124535,0.0000152345965,0.00006809401,0.00018425401,0.00016260718,0.028995654,0.048876066,0.00055190903,0.008442058,0.000023176237],"about_ca_topic_score_codex":0.001540785,"about_ca_topic_score_gemma":0.0036961196,"teacher_disagreement_score":0.0018578521,"about_ca_system_score_codex":0.00018764492,"about_ca_system_score_gemma":0.00007478972,"threshold_uncertainty_score":0.0062150955},"labels":[],"label_agreement":null},{"id":"W2799089586","doi":"10.3847/1538-4357/aac01e","title":"Extended Structures of Planetary Nebulae Detected in H<sub>2</sub> Emission<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Planetary nebula; Halo; Interstellar medium; Emission spectrum; Infrared; Galaxy; Telescope; Stars; H II region","score_opus":0.007782282835725863,"score_gpt":0.21648989484247574,"score_spread":0.2087076120067499,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2799089586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99708253,0.00015523114,0.00029593302,0.000015033176,0.0000035519581,0.000004856905,0.00069912634,0.000028473893,0.0017151219],"genre_scores_gemma":[0.9973335,0.00006375742,0.0005517221,0.000024145274,0.000012167619,0.0000061868777,0.0015194739,0.000011967753,0.00047710357],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996424,0.0000022616196,0.0000023944026,0.000010524908,0.000007756068,0.000012785606],"domain_scores_gemma":[0.9998505,0.00001785661,0.000052538184,0.00001423064,0.000023699657,0.000041153224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000091964066,0.0001654545,0.00010144025,0.0008742294,0.0001992665,0.00033572776,0.00014694167,0.00017246447,0.0029954324],"category_scores_gemma":[0.00013296684,0.00009396571,0.00010844222,0.00031795955,0.00015282443,0.000138659,0.00023501323,0.00011479733,0.0004592645],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057732343,0.000096253876,0.4791241,0.00009783952,0.000078905665,0.0023937859,0.00041409553,0.000346628,0.49489695,0.00017586912,0.0013902744,0.020408006],"study_design_scores_gemma":[0.0000016569882,0.0000234758,0.9932573,0.000002491736,0.000008971648,0.0007139029,0.00007714747,0.0001124333,0.005096167,0.000020413914,0.00068367855,0.0000022913348],"about_ca_topic_score_codex":0.0012513471,"about_ca_topic_score_gemma":0.0019885756,"teacher_disagreement_score":0.0029954324,"about_ca_system_score_codex":0.00008580946,"about_ca_system_score_gemma":0.00004714765,"threshold_uncertainty_score":0.010020733},"labels":[],"label_agreement":null},{"id":"W2799187493","doi":"10.3847/1538-4357/aabd82","title":"A First Look at BISTRO Observations of the ρ Oph-A core","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Dalhousie University; University of Manitoba; Western University; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; East Asian Core Observatories Association; National Astronomical Observatory of Japan; Ministry of Education, Culture, Sports, Science and Technology; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; Korea Astronomy and Space Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Academia Sinica; Chinese Academy of Sciences; Ministry of Science, ICT and Future Planning; Science and Technology Facilities Council; National Research Foundation","keywords":"Physics; Polarization (electrochemistry); Sky; Polarimetry; Astrophysics; Magnetic field; Polarimeter; Faraday effect; Infrared; Astronomy; Optics; Scattering","score_opus":0.030622413987381532,"score_gpt":0.2499622494891998,"score_spread":0.21933983550181826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2799187493","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931912,0.00017167251,0.0009308618,0.000046932117,0.000009343892,0.000008522498,0.0008491325,0.00007860969,0.0047137714],"genre_scores_gemma":[0.9976446,0.00005161638,0.00078885705,0.00004280483,0.000019986273,0.0000039437696,0.0011778438,0.000010327441,0.0002599925],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999229,0.000006927051,0.0000035535868,0.000019369289,0.00002508911,0.00002217206],"domain_scores_gemma":[0.99970007,0.000030453322,0.00006588924,0.000036440346,0.000053665182,0.00011353002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015387767,0.00017789689,0.00016364123,0.0009898108,0.00030864013,0.00040659093,0.0002341798,0.00021081309,0.0013409761],"category_scores_gemma":[0.00031490266,0.00013376152,0.00011729075,0.00056785345,0.00017283636,0.00026801636,0.00053786434,0.00025605134,0.00026441904],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048028247,0.00023095841,0.64823556,0.00008430123,0.00012860252,0.0007629813,0.000637652,0.0010290699,0.30014652,0.0010749382,0.0025802234,0.044608925],"study_design_scores_gemma":[0.000009939274,0.000051631472,0.9925916,0.000008395778,0.00001712487,0.0001917912,0.000095637,0.00095052476,0.0037949572,0.00015425104,0.0021280583,0.0000060793504],"about_ca_topic_score_codex":0.0023685836,"about_ca_topic_score_gemma":0.005155481,"teacher_disagreement_score":0.0023685836,"about_ca_system_score_codex":0.00015699494,"about_ca_system_score_gemma":0.000098249744,"threshold_uncertainty_score":0.004709542},"labels":[],"label_agreement":null},{"id":"W2799200053","doi":"10.3847/1538-4357/aabe8e","title":"A Thorough View of the Nuclear Region of NGC 253: Combined Herschel, SOFIA, and APEX Data Set","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Radiative transfer; Spire (mollusc); Spectral line; On board; Galaxy; Spectral energy distribution; Spectral signature; Photometry (optics); Line (geometry)","score_opus":0.031451555336362604,"score_gpt":0.26798776351143627,"score_spread":0.23653620817507368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2799200053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8225081,0.000257128,0.0008052127,0.000098427045,0.000009749826,0.000026071542,0.17223068,0.00062983186,0.0034347747],"genre_scores_gemma":[0.71338314,0.00016074709,0.0030157592,0.000059528684,0.000019006671,0.00006023637,0.28205964,0.00014576291,0.0010962],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962056,0.000029674839,0.000035104,0.00012534067,0.000111116125,0.000078166835],"domain_scores_gemma":[0.9991743,0.00009172138,0.000113789334,0.00031550927,0.00017776668,0.00012692617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004867156,0.00038574444,0.00053733634,0.0018449594,0.0003630636,0.00077664043,0.00050191884,0.00031698644,0.003325202],"category_scores_gemma":[0.0007515677,0.00015940954,0.0005102008,0.0015193267,0.00016411659,0.00042748573,0.00056078477,0.0002715937,0.0019922946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036288192,0.00022049776,0.8480947,0.00018694674,0.0004731311,0.0010148161,0.00040585618,0.01895163,0.030868823,0.0008251301,0.035278752,0.06331692],"study_design_scores_gemma":[0.000035495712,0.00004328754,0.96918327,0.000026777756,0.000055229968,0.00017314455,0.00026500045,0.007962622,0.0034738993,0.00015946367,0.018591544,0.000030237909],"about_ca_topic_score_codex":0.055301026,"about_ca_topic_score_gemma":0.066517815,"teacher_disagreement_score":0.055301026,"about_ca_system_score_codex":0.00082731573,"about_ca_system_score_gemma":0.0006666537,"threshold_uncertainty_score":0.10995823},"labels":[],"label_agreement":null},{"id":"W2799267490","doi":"10.3847/1538-4357/aac1b8","title":"The Next Generation Fornax Survey (NGFS). IV. Mass and Age Bimodality of Nuclear Clusters in the Fornax Core Region","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Fornax Cluster; Stellar mass; Stellar population; Surface brightness; Population; Star formation","score_opus":0.044191054995727876,"score_gpt":0.24616443043033026,"score_spread":0.2019733754346024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2799267490","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959409,0.00017296567,0.00006953218,0.00003022001,0.000002494554,0.0000072435946,0.0017022765,0.000015306592,0.0020590145],"genre_scores_gemma":[0.9920609,0.000096202064,0.000361319,0.000017807646,0.000007509603,0.000013639722,0.0051610093,0.000008741894,0.0022730273],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998677,0.000019619507,0.000006316001,0.000047022844,0.00002714268,0.000032138494],"domain_scores_gemma":[0.9996939,0.00002226119,0.00011228041,0.000042728057,0.000051770814,0.000077182296],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030298237,0.00015560859,0.00012756501,0.0007715689,0.00022523031,0.00025368237,0.00022595968,0.00013332882,0.0020218138],"category_scores_gemma":[0.00046213352,0.00006594603,0.00013946815,0.0003405053,0.00013858604,0.00029720605,0.00050110713,0.000085756204,0.000468034],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005486751,0.0000070736696,0.989954,0.000013843195,0.00001929695,0.000042971315,0.00031427114,0.000074472366,0.002282998,0.0001220623,0.0005678555,0.0065462193],"study_design_scores_gemma":[0.0000010920461,0.000009715188,0.9987558,0.0000028053512,0.0000024048613,0.000034690904,0.00006256433,0.000059543683,0.00010218097,0.00001215475,0.000956353,7.74655e-7],"about_ca_topic_score_codex":0.019166682,"about_ca_topic_score_gemma":0.03199655,"teacher_disagreement_score":0.019166682,"about_ca_system_score_codex":0.0004119392,"about_ca_system_score_gemma":0.00018088627,"threshold_uncertainty_score":0.038110256},"labels":[],"label_agreement":null},{"id":"W2799383556","doi":"10.3847/1538-4357/aac3e2","title":"Protoplanetary Disk Properties in the Orion Nebula Cluster: Initial Results from Deep, High-resolution ALMA Observations","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":143,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Orion Nebula; Millimeter; Submillimeter Array; Flux (metallurgy); Protoplanetary disk; Nebula; Young stellar object; Cluster (spacecraft); Circumstellar disk; Angular resolution (graph drawing)","score_opus":0.03039455243341695,"score_gpt":0.2440203545646808,"score_spread":0.21362580213126384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2799383556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943644,0.00005504918,0.0000827057,0.000005860768,6.745165e-7,0.0000026608914,0.00019799125,0.0000063294938,0.00021214214],"genre_scores_gemma":[0.9986921,0.000031487183,0.0004023247,0.000007614036,0.000004907475,0.000002742002,0.0006503318,0.0000041886965,0.00020433964],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986994,0.000011911395,0.000006060512,0.000047994683,0.0000348963,0.00002910714],"domain_scores_gemma":[0.9995844,0.000058318798,0.00008064389,0.00005887999,0.000101922524,0.00011592085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003155825,0.00025522948,0.00020758618,0.0005591156,0.00039012398,0.0004870131,0.00025752693,0.00020072705,0.00041160552],"category_scores_gemma":[0.00051005225,0.00013267074,0.00015378541,0.00040894773,0.00021888726,0.0002960395,0.00041746002,0.00017956427,0.00015526621],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020585896,0.000082575614,0.9676781,0.000020474597,0.000048775026,0.00018369536,0.000577755,0.0005632126,0.022985969,0.000053101394,0.00020896523,0.007391594],"study_design_scores_gemma":[0.0000027530784,0.000015321562,0.99885905,0.0000012128231,0.000007016836,0.000033191325,0.000074960546,0.0003991204,0.0004001565,0.000010685223,0.00019396337,0.0000024411402],"about_ca_topic_score_codex":0.01126652,"about_ca_topic_score_gemma":0.02382676,"teacher_disagreement_score":0.01126652,"about_ca_system_score_codex":0.00039522312,"about_ca_system_score_gemma":0.00012821086,"threshold_uncertainty_score":0.022401929},"labels":[],"label_agreement":null},{"id":"W2800477370","doi":"10.3847/1538-4357/aac2ec","title":"Infall Signatures in a Prestellar Core Embedded in the High-mass 70 μm Dark IRDC G331.372-00.116","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Star formation; Accretion (finance); Virial theorem; Molecular cloud; Infrared; Core (optical fiber); Basso continuo; Submillimeter Array","score_opus":0.01144079715224533,"score_gpt":0.2511302051061802,"score_spread":0.2396894079539349,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2800477370","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997706,0.000011966911,0.000014194439,0.0000022909142,3.3498938e-7,0.0000012386425,0.000049642025,0.0000019771605,0.00014769379],"genre_scores_gemma":[0.99968565,0.000005308507,0.000045720466,0.0000064761302,7.9842226e-7,8.903732e-7,0.00016663816,9.969083e-7,0.00008749307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995637,0.0000025862469,0.0000014585771,0.000011889963,0.0000090134345,0.000018619092],"domain_scores_gemma":[0.9998498,0.000006479121,0.000046458543,0.0000088186225,0.000015237084,0.00007310927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000060499133,0.00017722746,0.00016797853,0.00031654284,0.00031202595,0.00028008624,0.00020549203,0.00012358451,0.00053252815],"category_scores_gemma":[0.000084704916,0.00008547242,0.00007036134,0.00019575773,0.00017355738,0.00007947291,0.00027772947,0.00015121774,0.00012229162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043282707,0.000111504036,0.76023793,0.00002165312,0.00003278725,0.0010208379,0.00030887095,0.0003049575,0.23399988,0.000094748735,0.00018546799,0.0032486562],"study_design_scores_gemma":[0.0000044716053,0.000058643014,0.99689144,0.0000011496525,0.0000053740177,0.00013433956,0.000111499685,0.0002574261,0.0023479664,0.0000067993324,0.00017960939,0.0000013894409],"about_ca_topic_score_codex":0.011280264,"about_ca_topic_score_gemma":0.019810194,"teacher_disagreement_score":0.011280264,"about_ca_system_score_codex":0.00033930826,"about_ca_system_score_gemma":0.00008837098,"threshold_uncertainty_score":0.022429228},"labels":[],"label_agreement":null},{"id":"W2800639241","doi":"10.3847/1538-4357/aab1fd","title":"A-type Stellar Abundances: A Corollary to Herschel Observations of Debris Disks","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Stars; Astrophysics; Metallicity; Planetesimal; Debris disk; Astronomy; Lambda; Planetary system; Abundance (ecology); Planet","score_opus":0.030024739968332815,"score_gpt":0.26100407031442957,"score_spread":0.23097933034609675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2800639241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9890822,0.00023331074,0.0021789458,0.00010875929,0.000011010414,0.000009076226,0.0013218578,0.00005097382,0.007004003],"genre_scores_gemma":[0.9981888,0.00004184855,0.00082457525,0.00003941624,0.000017805169,0.0000039821216,0.00036484379,0.00000718138,0.0005114645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999616,0.000043978373,0.000029361057,0.0001425004,0.00012985853,0.000038254067],"domain_scores_gemma":[0.9977633,0.00039081328,0.00088828703,0.00039667785,0.0003845496,0.00017640754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005603146,0.00016643506,0.00018261283,0.0006101947,0.00035954823,0.0007273486,0.0003053463,0.0002973744,0.0028291203],"category_scores_gemma":[0.002310694,0.000101701866,0.00014066361,0.0005815485,0.0003191032,0.00059872726,0.00051349745,0.00022379929,0.00080540444],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000081234764,0.00002289427,0.9753009,0.00003373289,0.000038692284,0.000032118085,0.00009247586,0.0003603085,0.014939452,0.0006200243,0.00022647352,0.008251785],"study_design_scores_gemma":[0.0000047433196,0.000035949437,0.9950765,0.0000070112546,0.000007689444,0.00013878745,0.00008049264,0.001028985,0.0018758682,0.0006505864,0.0010901674,0.0000032415062],"about_ca_topic_score_codex":0.002062189,"about_ca_topic_score_gemma":0.0027721701,"teacher_disagreement_score":0.0028291203,"about_ca_system_score_codex":0.00021338566,"about_ca_system_score_gemma":0.00009738415,"threshold_uncertainty_score":0.009464383},"labels":[],"label_agreement":null},{"id":"W2801102073","doi":"10.3847/1538-4357/aab8f2","title":"A Solar-flux Line-broadening Analysis","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Flux (metallurgy); Astrophysics; Line (geometry); Solar rotation; Spectral line; Radial velocity; Rotation (mathematics); Fourier transform; Computational physics; Fourier analysis; Solar physics; Stellar rotation; Residual; Stellar atmosphere; Optics; Stars; Astronomy; Geometry","score_opus":0.008204360606201068,"score_gpt":0.24640926789324513,"score_spread":0.23820490728704408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2801102073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8639169,0.00041655282,0.09765854,0.00009816739,0.000063001244,0.00008260865,0.002768466,0.002495674,0.03250013],"genre_scores_gemma":[0.97327155,0.00013338728,0.022304095,0.000029940193,0.00002429802,0.000021646194,0.0014454906,0.00016619734,0.0026034792],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992144,0.0000073272995,0.0000031549475,0.000026649655,0.00003278342,0.000008641174],"domain_scores_gemma":[0.9998641,0.000021652751,0.00002007045,0.00002593186,0.000056547342,0.000011787248],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020552674,0.00019255403,0.00013221585,0.0016873667,0.00029632048,0.00030774396,0.00026340602,0.00021449839,0.00366523],"category_scores_gemma":[0.000376497,0.00008670991,0.00031285494,0.0006660282,0.00006691538,0.00029404546,0.00021666693,0.00021099245,0.00095615094],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004694935,0.00026248963,0.11666501,0.0001807366,0.00016005337,0.00038358537,0.0002536578,0.01307412,0.4938945,0.007496113,0.0059014484,0.3612589],"study_design_scores_gemma":[0.000059089467,0.00021621388,0.6163954,0.0000452461,0.000109801156,0.0009545875,0.00015303362,0.1973021,0.14579774,0.0037689966,0.035127714,0.000070027556],"about_ca_topic_score_codex":0.0012808638,"about_ca_topic_score_gemma":0.0011634119,"teacher_disagreement_score":0.00366523,"about_ca_system_score_codex":0.00020823661,"about_ca_system_score_gemma":0.000116103416,"threshold_uncertainty_score":0.01226145},"labels":[],"label_agreement":null},{"id":"W2801402560","doi":"10.3847/1538-4357/aac324","title":"Star Formation Histories of z ∼ 1 Galaxies in LEGA-C","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Star formation; Galaxy formation and evolution; Cosmic time; Redshift; Peculiar galaxy; Luminous infrared galaxy; Stars","score_opus":0.008358580886234052,"score_gpt":0.21135304986134704,"score_spread":0.20299446897511297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2801402560","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99668115,0.000052265714,0.00014048739,0.0000194783,0.0000010359029,0.0000034260565,0.0025671262,0.000028777373,0.0005061832],"genre_scores_gemma":[0.99282324,0.000026144073,0.00032793783,0.000016800497,0.0000018593289,0.000004170317,0.0065797693,0.000008352196,0.00021165039],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998958,0.000014911399,0.0000056523445,0.000037897902,0.000016235812,0.000029530034],"domain_scores_gemma":[0.9994135,0.00011676928,0.00020343185,0.00006992696,0.00006886275,0.00012745442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020013271,0.00017564908,0.0001652248,0.0017427929,0.0002093764,0.0007423646,0.0002730005,0.00024761976,0.0012155506],"category_scores_gemma":[0.0009599682,0.000103622835,0.000261919,0.0009380124,0.00017276287,0.00021255066,0.00044439858,0.00017563601,0.00041979735],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005940494,0.000016078058,0.991751,0.000008190586,0.000043457276,0.000046838682,0.00016488254,0.0010903263,0.0021119905,0.0001696154,0.00030895643,0.004229275],"study_design_scores_gemma":[0.000002884767,0.000008099299,0.9969842,0.0000027151045,0.000005860963,0.00003745324,0.000038007107,0.0021391439,0.00024000897,0.00005888093,0.0004797118,0.0000030623196],"about_ca_topic_score_codex":0.024008133,"about_ca_topic_score_gemma":0.030822279,"teacher_disagreement_score":0.024008133,"about_ca_system_score_codex":0.00062176515,"about_ca_system_score_gemma":0.00015371828,"threshold_uncertainty_score":0.047736764},"labels":[],"label_agreement":null},{"id":"W2802133844","doi":"10.3847/1538-4357/aabf8a","title":"The Green Bank North Celestial Cap Pulsar Survey. III. 45 New Pulsar Timing Solutions","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Precursory Research for Embryonic Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Discovery Communications; Canada Research Chairs; Natural Sciences and Engineering Research Council of Canada; European Commission; Northern Arizona University; National Science Foundation","keywords":"Pulsar; Millisecond pulsar; Green Bank Telescope; Neutron star; Binary pulsar; Proper motion; Gravitational wave; Binary number","score_opus":0.03463905372383097,"score_gpt":0.3207757023115344,"score_spread":0.28613664858770343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2802133844","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92686343,0.0024219404,0.0027946439,0.00047267298,0.00014258908,0.00016282695,0.051049072,0.00033297652,0.015759898],"genre_scores_gemma":[0.8832957,0.0019094136,0.009377925,0.00040919974,0.00028631333,0.00024918668,0.09446051,0.0001235981,0.009888159],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994054,0.000083247796,0.00006881328,0.000108744396,0.00021453647,0.00011917249],"domain_scores_gemma":[0.9979436,0.00024321418,0.0005336792,0.00031480135,0.0005419428,0.00042275313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00095491856,0.00032411187,0.00030985952,0.004109549,0.00044634772,0.0010726394,0.00039905746,0.00025809868,0.0035797444],"category_scores_gemma":[0.0016752381,0.00022393887,0.00016530706,0.0038333575,0.00020678376,0.00038318857,0.0008073378,0.00032073617,0.0016111925],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025997637,0.00003829933,0.9195581,0.00007637273,0.0000573874,0.00024088891,0.00027741643,0.000458592,0.003612247,0.00034310107,0.011881214,0.06319633],"study_design_scores_gemma":[0.00003086493,0.000036479138,0.9684174,0.000028824476,0.000022813652,0.00017208017,0.00015244381,0.000771561,0.000702242,0.00010197998,0.02955252,0.000010847594],"about_ca_topic_score_codex":0.05620701,"about_ca_topic_score_gemma":0.13837007,"teacher_disagreement_score":0.05620701,"about_ca_system_score_codex":0.0009048432,"about_ca_system_score_gemma":0.000924128,"threshold_uncertainty_score":0.11175966},"labels":[],"label_agreement":null},{"id":"W2802975680","doi":"10.3847/1538-4357/aac438","title":"Molecular Gas Contents and Scaling Relations for Massive, Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Star formation; Galaxy; Luminous infrared galaxy; Astronomy; Redshift; Accretion (finance); Peculiar galaxy; Lenticular galaxy","score_opus":0.012456526218757697,"score_gpt":0.226709967675342,"score_spread":0.2142534414565843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2802975680","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983101,0.00009364722,0.00006577842,0.000021532063,0.0000014044457,0.0000025273682,0.00091438554,0.000011118014,0.00057961605],"genre_scores_gemma":[0.99878997,0.000028124188,0.000053202428,0.000008897694,0.000003659094,0.0000017044887,0.0010390858,0.0000027904405,0.00007254835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998498,0.000020479583,0.000012094575,0.000056768666,0.000022112077,0.000038750357],"domain_scores_gemma":[0.9987531,0.00022217844,0.00052069157,0.00011694167,0.00012194058,0.0002652874],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002763689,0.00021850274,0.0002035888,0.0028572893,0.00025910907,0.0008606296,0.00032975478,0.00031143602,0.0016357906],"category_scores_gemma":[0.0009127246,0.000121390156,0.0002495464,0.0010893621,0.00032184838,0.0003732782,0.0005047166,0.00020380886,0.0003619996],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031280735,0.000007418695,0.9973894,0.000004269651,0.000020903162,0.000018047598,0.000081371145,0.000048964932,0.0013890542,0.000041663297,0.00006794018,0.00089982],"study_design_scores_gemma":[9.98024e-7,0.0000045131883,0.99967706,0.0000011629468,0.0000036319448,0.000017980245,0.000039224444,0.00010393141,0.00006149551,0.000012049845,0.0000770839,8.7743405e-7],"about_ca_topic_score_codex":0.010199215,"about_ca_topic_score_gemma":0.012244619,"teacher_disagreement_score":0.010199215,"about_ca_system_score_codex":0.0003512899,"about_ca_system_score_gemma":0.00008775285,"threshold_uncertainty_score":0.020279706},"labels":[],"label_agreement":null},{"id":"W2803459877","doi":"10.3847/1538-4357/ab90fb","title":"Rotation, Convective Core Overshooting, and Period Changes in Classical Cepheid Stellar Evolution Models","year":2020,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia","funders":"","keywords":"Cepheid variable; Physics; Astrophysics; Stellar evolution; Stellar rotation; Rotation (mathematics); Rotation period; Convection; Stars; Luminosity; Period (music); Stellar structure; Astronomy; Mechanics","score_opus":0.027370686565726634,"score_gpt":0.24383565833090884,"score_spread":0.2164649717651822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2803459877","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960328,0.00011026253,0.0024225232,0.00009555266,0.0000048536244,0.0000055878995,0.00018028752,0.000015636555,0.0011324949],"genre_scores_gemma":[0.99929047,0.00004553859,0.00029680337,0.000008276829,0.000007542582,0.0000034415314,0.00010965787,0.0000036863837,0.00023461285],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998492,0.000055628487,0.000008075597,0.00003832818,0.000017254592,0.00003147629],"domain_scores_gemma":[0.9990252,0.00048077456,0.00019413499,0.00009477324,0.000058708592,0.00014641994],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009153281,0.00027876487,0.00033291103,0.0005928311,0.00032799493,0.0010663318,0.0007698125,0.00037430163,0.0015311342],"category_scores_gemma":[0.0022158497,0.0001301375,0.00028733554,0.00038945308,0.00069553166,0.0004593265,0.00043118428,0.00025043805,0.00015970286],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067247613,0.00016682106,0.26822543,0.00007304579,0.00017293656,0.00043700304,0.0003475472,0.69175595,0.002483546,0.023652704,0.0013421751,0.0106704505],"study_design_scores_gemma":[0.00003843535,0.000056542824,0.05599562,0.000008795912,0.000031035284,0.00006721687,0.00006582324,0.9371444,0.00026879928,0.0058334963,0.00047713172,0.000012786657],"about_ca_topic_score_codex":0.012376974,"about_ca_topic_score_gemma":0.0059971428,"teacher_disagreement_score":0.012376974,"about_ca_system_score_codex":0.00089861976,"about_ca_system_score_gemma":0.00019343989,"threshold_uncertainty_score":0.024609864},"labels":[],"label_agreement":null},{"id":"W2803715449","doi":"10.3847/1538-4357/aadae2","title":"The Impact of Vector Resonant Relaxation on the Evolution of Binaries near a Massive Black Hole: Implications for Gravitational-wave Sources","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"LIGO; Physics; Gravitational wave; Astrophysics; Black hole (networking); Binary number; Monte Carlo method; Galactic Center; Relaxation (psychology); Stars; Statistics","score_opus":0.0209851758780463,"score_gpt":0.3319333607818705,"score_spread":0.3109481849038242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2803715449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975193,0.00008884447,0.00081544596,0.00012841103,0.000007262544,0.000005484843,0.000075004355,0.000019605093,0.0013406876],"genre_scores_gemma":[0.9996203,0.000026578236,0.00017028356,0.000016430737,0.0000035183707,0.00000240317,0.00003233524,0.0000066119355,0.000121425124],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991333,0.000029599069,0.0000041224134,0.000013532558,0.000010794324,0.000028499559],"domain_scores_gemma":[0.9991297,0.00042302517,0.00015431567,0.000048517166,0.000052288844,0.00019215081],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004992178,0.00034401813,0.00055750797,0.0004346794,0.0006905158,0.001151103,0.0006060824,0.0008079889,0.0023090523],"category_scores_gemma":[0.0018270036,0.0002913406,0.0005109035,0.00024970443,0.0005904774,0.0007966631,0.0007421683,0.0005900386,0.000183261],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003545191,0.00025457196,0.10412292,0.00005642991,0.00018104147,0.0006350618,0.00011719822,0.8751114,0.008752694,0.0071105375,0.00042459162,0.0028789605],"study_design_scores_gemma":[0.000050918712,0.00012130903,0.025402226,0.000010414441,0.000046935096,0.00007872618,0.000097184755,0.97081393,0.0015356117,0.0016174482,0.00019669696,0.00002856281],"about_ca_topic_score_codex":0.0067488337,"about_ca_topic_score_gemma":0.0035225716,"teacher_disagreement_score":0.0067488337,"about_ca_system_score_codex":0.0007569914,"about_ca_system_score_gemma":0.00038595631,"threshold_uncertainty_score":0.013419092},"labels":[],"label_agreement":null},{"id":"W2803836611","doi":"10.3847/1538-4357/aac5e5","title":"An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Number Counts of Submillimeter Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"National Institutes of Natural Sciences; Chinese Academy of Sciences; European Commission; Academia Sinica; National Science Council; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Narodowym Centrum Nauki; National Science Foundation","keywords":"Submillimeter Array; Galaxy; Cosmology; Luminosity; Source counts; Millimeter; Luminous infrared galaxy; Photometry (optics)","score_opus":0.015459082230272408,"score_gpt":0.2574253405434136,"score_spread":0.2419662583131412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2803836611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9754072,0.00024967748,0.0015727633,0.000086573324,0.000015368494,0.000053941578,0.016109504,0.00028796497,0.006217084],"genre_scores_gemma":[0.96682477,0.0001462512,0.0040550805,0.00009485441,0.000061532286,0.000075292344,0.025119686,0.00008029312,0.0035422305],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993299,0.00014959685,0.000034084893,0.00014096627,0.00024130827,0.00010405685],"domain_scores_gemma":[0.9979183,0.00021880884,0.0003904009,0.00040128062,0.0006225009,0.00044860537],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006037609,0.00025051043,0.00023397827,0.0030004692,0.00031884652,0.00061249535,0.00043045002,0.00018053922,0.0032849747],"category_scores_gemma":[0.0012927024,0.000166092,0.00022294249,0.0021439989,0.00019789491,0.00036189455,0.00071993005,0.00018300502,0.0013808609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002036626,0.000063372136,0.952289,0.000056218058,0.000075893404,0.00010054837,0.00031862274,0.00043927168,0.010444484,0.00037829395,0.010515118,0.025115395],"study_design_scores_gemma":[0.000010983955,0.000018621686,0.9930568,0.000008193499,0.000010704451,0.00004323721,0.000054538763,0.00050645036,0.0012556991,0.000041157025,0.0049871583,0.000006433604],"about_ca_topic_score_codex":0.018852713,"about_ca_topic_score_gemma":0.036802556,"teacher_disagreement_score":0.018852713,"about_ca_system_score_codex":0.0004715199,"about_ca_system_score_gemma":0.0002896437,"threshold_uncertainty_score":0.037485957},"labels":[],"label_agreement":null},{"id":"W2803920522","doi":"10.3847/1538-4357/aac4a2","title":"A Very High Energy γ-Ray Survey toward the Cygnus Region of the Galaxy","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Crab Nebula; Pulsar; Galaxy; Supernova remnant; Telescope; Supernova; Pulsar wind nebula; High energy; Nebula","score_opus":0.014113785713009391,"score_gpt":0.2115256864091278,"score_spread":0.19741190069611841,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2803920522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99894804,0.000074961936,0.00013612263,0.000011957339,9.150204e-7,0.0000030284252,0.00026847128,0.000016176227,0.00054034055],"genre_scores_gemma":[0.9982054,0.00007094479,0.00034954256,0.0000146120965,0.000004600427,0.0000037304524,0.001042483,0.0000063918856,0.00030222346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999871,0.000015223957,0.0000055039327,0.00003512629,0.000030582698,0.00004254864],"domain_scores_gemma":[0.9996419,0.000047739813,0.00009888759,0.00004979641,0.00005070413,0.00011095203],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021919403,0.0002263064,0.0001861677,0.0015990203,0.00031406467,0.00048961694,0.00016647903,0.00015936895,0.00062592357],"category_scores_gemma":[0.0002760205,0.00013773433,0.00018834021,0.0009199945,0.00025485014,0.00014427128,0.0005753307,0.00015865089,0.00015232671],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019225832,0.00003745126,0.9295978,0.000022935412,0.00010198266,0.00045341256,0.00036867312,0.0005863383,0.055212483,0.0001548881,0.00035269166,0.012918956],"study_design_scores_gemma":[0.0000027885037,0.000021965936,0.9981129,0.0000027216074,0.000010381081,0.000119142154,0.000059597303,0.00020488772,0.0009137808,0.00001997528,0.0005290727,0.000002660753],"about_ca_topic_score_codex":0.01567226,"about_ca_topic_score_gemma":0.03208466,"teacher_disagreement_score":0.01567226,"about_ca_system_score_codex":0.00049404206,"about_ca_system_score_gemma":0.0002599293,"threshold_uncertainty_score":0.031162083},"labels":[],"label_agreement":null},{"id":"W2804244417","doi":"10.3847/1538-4357/aac512","title":"The MALATANG Survey: The L<sub>GAS</sub>–L<sub>IR</sub>Correlation on Sub-kiloparsec Scale in Six Nearby Star-forming Galaxies as Traced by HCN J = 4 → 3 and HCO<sup>+</sup>J = 4 → 3","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Alberta; University of Toronto; McMaster University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Star formation; Luminosity; Luminous infrared galaxy; Infrared; Flux (metallurgy); Astronomy","score_opus":0.006751056251697992,"score_gpt":0.2051283952125684,"score_spread":0.1983773389608704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804244417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989894,0.000050952865,0.000040651226,0.000023663624,9.580624e-7,0.0000020252955,0.0003897231,0.000007917376,0.00049472094],"genre_scores_gemma":[0.9987552,0.000050578154,0.000120563534,0.000017870625,0.000004640124,0.000004170645,0.0007452378,0.0000026848163,0.00029902434],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998914,0.000014694511,0.000005657486,0.000040777977,0.000018869872,0.000028677046],"domain_scores_gemma":[0.99945813,0.000050261173,0.00027243167,0.000055651024,0.00005184813,0.00011169448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000121110825,0.00016036742,0.00013903301,0.00093342585,0.00029288765,0.0004772282,0.00025585442,0.00017041816,0.001223827],"category_scores_gemma":[0.00034246626,0.00011752115,0.00013558658,0.00065990636,0.00024792473,0.00022715748,0.0005045593,0.00017186152,0.00031565982],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047450412,0.000008542936,0.9922317,0.0000103310485,0.000020112742,0.0000627843,0.00023653048,0.000044142897,0.005113719,0.00003663314,0.00013583282,0.0020521504],"study_design_scores_gemma":[0.0000010592688,0.000004094501,0.9994462,0.0000010218278,0.0000038760786,0.000024503412,0.000069650116,0.000037116944,0.00013852518,0.0000032023195,0.00026986047,8.597828e-7],"about_ca_topic_score_codex":0.018105047,"about_ca_topic_score_gemma":0.04930546,"teacher_disagreement_score":0.018105047,"about_ca_system_score_codex":0.00044993797,"about_ca_system_score_gemma":0.00013960812,"threshold_uncertainty_score":0.035999358},"labels":[],"label_agreement":null},{"id":"W2804413181","doi":"10.3847/1538-4357/aabe2e","title":"Detection of Intrinsic Source Structure at ∼3 Schwarzschild Radii with Millimeter-VLBI Observations of SAGITTARIUS A*","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Smithsonian Institution; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Academia Sinica; European Southern Observatory; Generalitat Valenciana; National Science Foundation","keywords":"Very-long-baseline interferometry; Supermassive black hole; Schwarzschild radius; Sagittarius A*; Galactic Center; Context (archaeology); Brightness; Amplitude; Flux (metallurgy)","score_opus":0.010312161825202823,"score_gpt":0.20306051820931825,"score_spread":0.19274835638411542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804413181","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99876153,0.0000449278,0.00037820416,0.000018716983,0.0000017009977,0.0000021826334,0.00022674423,0.000031267777,0.000534681],"genre_scores_gemma":[0.9990545,0.000015982947,0.00042600243,0.000009033872,0.000004284127,0.000002037268,0.00043230387,0.0000042650977,0.000051512117],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989057,0.000017928343,0.0000068277855,0.000029663555,0.000030978405,0.000023990504],"domain_scores_gemma":[0.99961215,0.00003711302,0.00014412845,0.000060999784,0.000049590013,0.00009600576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025993402,0.00019286603,0.00019724462,0.00058918406,0.00027922823,0.0005180197,0.00026947196,0.00022109447,0.0006188812],"category_scores_gemma":[0.0003940873,0.00015650678,0.00026518048,0.00031649604,0.00022078522,0.000189094,0.00039356112,0.0002170238,0.00019360633],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001785941,0.000043934644,0.907543,0.000024853987,0.00011444409,0.00016549988,0.00023417748,0.0008706962,0.0831334,0.0002459473,0.00037063676,0.0070746876],"study_design_scores_gemma":[0.0000042138795,0.000025181009,0.99687296,0.0000022685006,0.000012124202,0.00006113365,0.000041572766,0.0008201596,0.00182445,0.00006180015,0.000270019,0.000004178695],"about_ca_topic_score_codex":0.0034960166,"about_ca_topic_score_gemma":0.005757227,"teacher_disagreement_score":0.0034960166,"about_ca_system_score_codex":0.00034340573,"about_ca_system_score_gemma":0.000115537514,"threshold_uncertainty_score":0.006951332},"labels":[],"label_agreement":null},{"id":"W2804476062","doi":"10.3847/1538-4357/aac4a6","title":"Magnetic Fields toward Ophiuchus-B Derived from SCUBA-2 Polarization Measurements","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Dalhousie University; University of Manitoba; Western University; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Magnetic field; Polarimeter; James Clerk Maxwell Telescope; Polarization (electrochemistry); Bolometer; Field strength; Telescope; Polarimetry; Field (mathematics)","score_opus":0.02519044466249762,"score_gpt":0.2476566356401495,"score_spread":0.22246619097765188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804476062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962846,0.00004440947,0.0002971076,0.000009868457,0.0000022689073,0.00001027876,0.0016753513,0.00005859977,0.0016174292],"genre_scores_gemma":[0.99649733,0.000030396604,0.00055752706,0.000009557111,0.000006082916,0.000008707511,0.0027147082,0.000010086325,0.00016559138],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998716,0.000012557131,0.000006889382,0.00003557699,0.000038620525,0.000034764525],"domain_scores_gemma":[0.9995714,0.000032422307,0.00011752727,0.000035858116,0.00012984133,0.00011298273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013903462,0.00032113332,0.00013166404,0.001923246,0.00027247524,0.00040419973,0.0002288562,0.00017833455,0.00091403036],"category_scores_gemma":[0.00047040923,0.0001231482,0.0001458805,0.00086579577,0.00016130292,0.00020032113,0.00046072755,0.00018329106,0.00028336418],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023064429,0.000051236366,0.903173,0.000052028183,0.0000817098,0.00023689985,0.00023297478,0.0012179144,0.0837345,0.00013875414,0.00069551956,0.010154738],"study_design_scores_gemma":[0.000007047687,0.000013361258,0.99393696,0.000005061008,0.000008695738,0.00005215975,0.000072255905,0.0013245712,0.0040707206,0.000031647956,0.00047296964,0.000004480248],"about_ca_topic_score_codex":0.008450436,"about_ca_topic_score_gemma":0.009006714,"teacher_disagreement_score":0.008450436,"about_ca_system_score_codex":0.00029740133,"about_ca_system_score_gemma":0.00012362364,"threshold_uncertainty_score":0.01680255},"labels":[],"label_agreement":null},{"id":"W2804560386","doi":"10.3847/1538-4357/aabfef","title":"Differential Rotation in Solar-like Convective Envelopes: Influence of Overshoot and Magnetism","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Differential rotation; Convection; Convection zone; Magnetohydrodynamics; Mechanics; Geophysical fluid dynamics; Geophysics; Classical mechanics; Astrophysics; Magnetic field; Stars","score_opus":0.0039997472715417245,"score_gpt":0.2140865925185143,"score_spread":0.21008684524697258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804560386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970939,0.000055350738,0.0009283195,0.00007906933,0.000011331317,0.000009897546,0.00010091329,0.00006509937,0.0016561605],"genre_scores_gemma":[0.9994598,0.000016288786,0.0003167842,0.000014226151,0.0000028667553,0.0000040809678,0.000073271825,0.000014765893,0.00009797947],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987495,0.00003687578,0.0000084970625,0.000017739012,0.000023062721,0.00003897088],"domain_scores_gemma":[0.99963415,0.0001485678,0.000052547453,0.000046566365,0.00003819378,0.00007993022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025824268,0.00039399357,0.00049365795,0.00032436536,0.00046175838,0.0008195985,0.00048230734,0.0005013276,0.00092433364],"category_scores_gemma":[0.0013093038,0.0001855986,0.00050275464,0.0002798057,0.0006047633,0.00034657758,0.00066720607,0.00045818975,0.00009409752],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004666187,0.0002635443,0.037918944,0.000060551454,0.00012764349,0.00044600564,0.000182908,0.92984927,0.023644539,0.0013322363,0.00044693283,0.005260892],"study_design_scores_gemma":[0.00013409357,0.00018369628,0.015763512,0.000010020829,0.000027410515,0.00005142119,0.00009549908,0.9777144,0.0051624225,0.0003595251,0.00047602932,0.00002191269],"about_ca_topic_score_codex":0.007053699,"about_ca_topic_score_gemma":0.0033884288,"teacher_disagreement_score":0.007053699,"about_ca_system_score_codex":0.00045501025,"about_ca_system_score_gemma":0.000414748,"threshold_uncertainty_score":0.014025271},"labels":[],"label_agreement":null},{"id":"W2804561849","doi":"10.3847/1538-4357/aac5f0","title":"The Implementation of a Fast-folding Pipeline for Long-period Pulsar Searching in the PALFA Survey","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Concordia University; University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; Science and Technology Facilities Council; Fonds Québécois de la Recherche sur la Nature et les Technologies; McGill University; National Science Foundation; Compute Canada; Canarie; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Pulsar; Sensitivity (control systems); Pipeline (software); Observatory; Fast Fourier transform; Noise (video); Duty cycle; Radio telescope","score_opus":0.025219081486687223,"score_gpt":0.3931749666306575,"score_spread":0.36795588514397026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804561849","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3346334,0.00005189128,0.62842256,0.00016872124,0.000038393817,0.00019217496,0.0003081253,0.033602245,0.002582448],"genre_scores_gemma":[0.63598514,0.000024316487,0.36141753,0.00009355295,0.000009378534,0.0001538797,0.00045369842,0.0006047651,0.0012578132],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99970776,0.00007302739,0.00001881753,0.00007891431,0.00006551423,0.000055858392],"domain_scores_gemma":[0.9988071,0.0006045716,0.00008682122,0.00019826778,0.00024264585,0.00006057931],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008513757,0.00051170815,0.00021470855,0.00029218846,0.0004171376,0.00046242942,0.0011388898,0.00043064164,0.0026328405],"category_scores_gemma":[0.0030960196,0.00025600105,0.00029335046,0.0002702951,0.000426139,0.00075085403,0.00040979614,0.00045447313,0.00049140817],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002267226,0.0007922711,0.060582303,0.00027924668,0.00016826602,0.00055620406,0.00079053105,0.37923318,0.11997373,0.010053469,0.0125993835,0.41270426],"study_design_scores_gemma":[0.00007015306,0.000103005186,0.0028619089,0.0000070758615,0.000011560643,0.000043319247,0.000025462232,0.96288514,0.031500284,0.0007030318,0.0017717759,0.000017252778],"about_ca_topic_score_codex":0.009066473,"about_ca_topic_score_gemma":0.0054685613,"teacher_disagreement_score":0.009066473,"about_ca_system_score_codex":0.0006304991,"about_ca_system_score_gemma":0.0013968918,"threshold_uncertainty_score":0.018027365},"labels":[],"label_agreement":null},{"id":"W2804743409","doi":"10.3847/1538-4357/aac6ba","title":"An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: Identifying Candidate z ∼ 4.5 [C II] Emitters","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"National Institutes of Natural Sciences; National Science Foundation; Korea Astronomy and Space Science Institute; Narodowym Centrum Nauki; Science and Technology Facilities Council; National Astronomical Observatory of Japan; European Commission; National Radio Astronomy Observatory","keywords":"Physics; Submillimeter Array; Astrophysics; Galaxy; Luminous infrared galaxy; Millimeter; Sky; Emission spectrum; Cosmology; Astronomy; Star formation; Spectral line","score_opus":0.01762321952369191,"score_gpt":0.2655362636128741,"score_spread":0.24791304408918216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804743409","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99832326,0.000045546738,0.00014222345,0.000017444145,0.0000013202456,0.00000785713,0.00053181377,0.000019571426,0.0009108761],"genre_scores_gemma":[0.99731654,0.00003515101,0.0006204872,0.000025536667,0.000006860069,0.000007826334,0.0014633543,0.0000053870976,0.00051869627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972695,0.00004899271,0.000011776284,0.00005122287,0.00008626077,0.000074794494],"domain_scores_gemma":[0.99908984,0.00009765546,0.00024993697,0.000095456795,0.00022630517,0.00024072423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042555932,0.0001786804,0.00012368719,0.0018978356,0.00034627918,0.00046936536,0.00034270764,0.00015615246,0.00142084],"category_scores_gemma":[0.0007286397,0.000121483376,0.00012681284,0.00088586565,0.00016549711,0.00023693733,0.00044487286,0.00012775967,0.00044175165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007562151,0.000032962762,0.98445165,0.000011974342,0.000021737764,0.00009838761,0.00017095858,0.000118497504,0.008483314,0.00008962951,0.00082636,0.0056189396],"study_design_scores_gemma":[0.0000037170048,0.0000156263,0.9981419,0.0000028742463,0.0000060800808,0.00004669896,0.000074239855,0.00035341262,0.0006628386,0.000012237181,0.0006784057,0.000001986926],"about_ca_topic_score_codex":0.017000206,"about_ca_topic_score_gemma":0.0346375,"teacher_disagreement_score":0.017000206,"about_ca_system_score_codex":0.00030906178,"about_ca_system_score_gemma":0.00020736779,"threshold_uncertainty_score":0.03380251},"labels":[],"label_agreement":null},{"id":"W2804939926","doi":"10.3847/1538-4357/aac76d","title":"Assessing the Impact of Astrochemistry on Molecular Cloud Turbulence Statistics","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Bicoherence; Molecular cloud; Physics; Turbulence; Astrophysics; Statistical physics; Statistics; Spectral density; Mathematics; Meteorology; Stars","score_opus":0.011532995166436593,"score_gpt":0.3084780980764686,"score_spread":0.296945102910032,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2804939926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977191,0.000026821555,0.0015697228,0.00005599739,0.0000071311333,0.000008718902,0.00015725748,0.000077612436,0.0003776057],"genre_scores_gemma":[0.9991092,0.000011200973,0.00069687585,0.000012611163,0.0000021970138,0.0000036722492,0.00011305215,0.000015748252,0.00003551683],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99966395,0.0000992665,0.000028763063,0.00005991205,0.00007680296,0.00007144281],"domain_scores_gemma":[0.9971787,0.001806414,0.0003635189,0.00024666757,0.00023005674,0.00017471027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010175112,0.0004517981,0.00036938483,0.00040022703,0.00046370664,0.00090329786,0.0005282392,0.00057515525,0.00050383504],"category_scores_gemma":[0.0055467943,0.00025713365,0.0005060903,0.0004531747,0.0007714075,0.0006433498,0.00048395008,0.0005796794,0.00007195887],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023895827,0.00014664663,0.06287005,0.00002976294,0.00008369359,0.00010956293,0.00006057383,0.9244057,0.008250943,0.0012273146,0.00019479655,0.002382139],"study_design_scores_gemma":[0.000032578748,0.0001358335,0.014954116,0.0000043997507,0.000014069201,0.000016577,0.000033830984,0.98010075,0.004353324,0.0002528039,0.00008538038,0.000016449785],"about_ca_topic_score_codex":0.015687995,"about_ca_topic_score_gemma":0.007745346,"teacher_disagreement_score":0.015687995,"about_ca_system_score_codex":0.00070668804,"about_ca_system_score_gemma":0.0007179511,"threshold_uncertainty_score":0.031193376},"labels":[],"label_agreement":null},{"id":"W2805626905","doi":"10.3847/1538-4357/aaeed0","title":"Spectroscopic Confirmation of Five Galaxy Clusters at z &gt; 1.25 in the 2500 deg<sup>2</sup> SPT-SZ Survey","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Argonne National Laboratory; Jet Propulsion Laboratory; Space Telescope Science Institute; University of Chicago; Office of Science; National Aeronautics and Space Administration; California Institute of Technology; High Energy Physics; Gordon and Betty Moore Foundation; U.S. Department of Energy; National Science Foundation","keywords":"Galaxy cluster; Galaxy; Redshift; Cluster (spacecraft); Telescope; Very Large Telescope; Spectroscopy; Brightest cluster galaxy; Galaxy group","score_opus":0.01042782681006789,"score_gpt":0.23009700573346342,"score_spread":0.21966917892339552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2805626905","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99868435,0.000026629836,0.00015697669,0.000032187705,0.0000033433978,0.000007301677,0.00038493966,0.000022224272,0.0006821091],"genre_scores_gemma":[0.99838054,0.0000130322105,0.00030656997,0.000016015161,0.000005233519,0.000004579389,0.0010049487,0.000006916208,0.00026205764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996574,0.000016433494,0.000018981154,0.00008629863,0.000116787756,0.000104162056],"domain_scores_gemma":[0.99888986,0.000068425936,0.00029662755,0.00010225562,0.00019936787,0.0004435703],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041026832,0.00024770832,0.00029681556,0.0015349545,0.00081780966,0.0007128104,0.00060690776,0.00022484323,0.0017049506],"category_scores_gemma":[0.0008364274,0.00017298888,0.00020939577,0.00070819183,0.0004915529,0.00020335676,0.0008911666,0.00030358406,0.0006353547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020370317,0.00004826475,0.96553504,0.000017615032,0.000033986096,0.00043448407,0.0008421589,0.00027375465,0.022448732,0.00035795438,0.0011942275,0.008610029],"study_design_scores_gemma":[0.0000063162615,0.000029610823,0.99721587,0.00000251794,0.00001220437,0.00013007372,0.00020776862,0.00023573397,0.0013605308,0.00003634314,0.00075937895,0.0000035418516],"about_ca_topic_score_codex":0.010138869,"about_ca_topic_score_gemma":0.016950043,"teacher_disagreement_score":0.010138869,"about_ca_system_score_codex":0.0006783275,"about_ca_system_score_gemma":0.0003024049,"threshold_uncertainty_score":0.020159721},"labels":[],"label_agreement":null},{"id":"W2805639602","doi":"10.3847/1538-4357/aac271","title":"Probing Self-interacting Dark Matter with Disk Galaxies in Cluster Environments","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Dark matter; Astrophysics; Dark matter halo; Galaxy; Halo; Cold dark matter; Galaxy cluster; Cluster (spacecraft); Observable; Quantum mechanics","score_opus":0.004497809596920627,"score_gpt":0.19828038350971816,"score_spread":0.19378257391279755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2805639602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989347,0.000017858758,0.00056509493,0.000023010201,0.0000014029677,0.0000034580262,0.000025958803,0.000016860813,0.00041167813],"genre_scores_gemma":[0.9995964,0.0000065813483,0.0003244618,0.000004412541,9.980835e-7,0.0000014321927,0.000020178566,0.000003862063,0.000041720825],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998698,0.00004790007,0.0000051397337,0.000026172811,0.000019228608,0.000031715466],"domain_scores_gemma":[0.9985678,0.0006064338,0.00026013583,0.00015774349,0.000121401434,0.00028650495],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038899985,0.00031721892,0.00038557054,0.00048159005,0.0006431702,0.00073177984,0.00081828557,0.00056169525,0.0008817502],"category_scores_gemma":[0.0017632347,0.00030184438,0.00032315476,0.0004488867,0.0007568135,0.00066965865,0.0010873299,0.00037723512,0.00010330603],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046076247,0.00037430515,0.23883522,0.00006589445,0.00031008106,0.000675211,0.0006641415,0.7190379,0.025180032,0.010788195,0.00051402336,0.0030943246],"study_design_scores_gemma":[0.000073905896,0.00014602114,0.055216014,0.0000074558566,0.00003459014,0.000106241554,0.00028250975,0.93580806,0.004357474,0.0034718208,0.0004630096,0.000032871318],"about_ca_topic_score_codex":0.008393413,"about_ca_topic_score_gemma":0.0036188562,"teacher_disagreement_score":0.008393413,"about_ca_system_score_codex":0.0010155645,"about_ca_system_score_gemma":0.00031642456,"threshold_uncertainty_score":0.016689122},"labels":[],"label_agreement":null},{"id":"W2805739003","doi":"10.3847/1538-4357/aabfe2","title":"High-cadence Multi-color Observations of the Dwarf Nova KSP-OT-201503a by the KMTNet Supernova Program","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Nova (rocket); Supernova; Cadence; Dwarf nova; Astrophysics; Astronomy; White dwarf; Stars; Aerospace engineering","score_opus":0.03216475231587468,"score_gpt":0.2716902459123445,"score_spread":0.2395254935964698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2805739003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975788,0.00007485518,0.00034918857,0.000010358698,0.000007863351,0.0000129578475,0.0011884605,0.00003207783,0.0007455436],"genre_scores_gemma":[0.9961738,0.000036798472,0.00066472497,0.000019040612,0.000009074222,0.000008000873,0.0028454715,0.000009993979,0.00023309264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998374,0.000010234515,0.000012904712,0.000044047854,0.00005721838,0.000038193164],"domain_scores_gemma":[0.9995079,0.000024634921,0.00011088004,0.000057123856,0.00007166844,0.00022781243],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037770867,0.00028100554,0.000262497,0.0010660448,0.00046395024,0.00035406317,0.0003180999,0.0001774251,0.0004759625],"category_scores_gemma":[0.00025534947,0.00014691449,0.00033308213,0.00056297064,0.00015418568,0.00017789468,0.0005640758,0.00023838368,0.00022040558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025738362,0.00016537054,0.9242081,0.00003603315,0.00010575461,0.0008904017,0.00020869955,0.0002918183,0.063719615,0.00012344809,0.00067584845,0.009317698],"study_design_scores_gemma":[0.000004187029,0.00004740711,0.9970862,0.0000031156692,0.000013827974,0.00043890515,0.000037171998,0.00036546364,0.0014446871,0.000020822348,0.00053420506,0.0000040075297],"about_ca_topic_score_codex":0.0060880184,"about_ca_topic_score_gemma":0.017816843,"teacher_disagreement_score":0.0060880184,"about_ca_system_score_codex":0.00035912928,"about_ca_system_score_gemma":0.00021438247,"threshold_uncertainty_score":0.012105167},"labels":[],"label_agreement":null},{"id":"W2805765380","doi":"10.3847/1538-4357/aad776","title":"Glitch Rises as a Test for Rapid Superfluid Coupling in Neutron Stars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Physics; Glitch; Neutron star; Superfluidity; Astrophysics; Astronomy; Coupling (piping); Stars; Nuclear physics; Optics; Condensed matter physics","score_opus":0.016614519994431125,"score_gpt":0.32829662810896676,"score_spread":0.3116821081145356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2805765380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99289364,0.0000849876,0.0052642184,0.00006455184,0.000010600645,0.0000117404925,0.00018806745,0.00016110367,0.0013210826],"genre_scores_gemma":[0.9992644,0.000026143522,0.0005197555,0.0000066055736,0.0000018949648,0.0000038157937,0.00008633441,0.000013640793,0.00007746054],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994683,0.000008355867,0.0000034219554,0.000013099169,0.000019676132,0.000008591186],"domain_scores_gemma":[0.99976426,0.00010380387,0.00006117167,0.000025813704,0.000027478387,0.000017420312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027599023,0.00019970628,0.00017417507,0.0003296476,0.00020818261,0.0003325729,0.00037421047,0.00032907864,0.00078796135],"category_scores_gemma":[0.0010471895,0.00013994866,0.00028835423,0.00023420862,0.00030427863,0.00031330655,0.00040162477,0.00039231096,0.000094757626],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007067214,0.00026687272,0.35849476,0.0004958566,0.00028981265,0.0018712248,0.0009684867,0.40357104,0.17818083,0.016428804,0.0018021635,0.036923498],"study_design_scores_gemma":[0.000026872369,0.00026315948,0.19118452,0.00004137711,0.00003361928,0.00016624562,0.00019277788,0.77039164,0.032851063,0.0038037114,0.0010108923,0.0000341588],"about_ca_topic_score_codex":0.0023620136,"about_ca_topic_score_gemma":0.0015649213,"teacher_disagreement_score":0.0023620136,"about_ca_system_score_codex":0.0004094359,"about_ca_system_score_gemma":0.00011815117,"threshold_uncertainty_score":0.004696548},"labels":[],"label_agreement":null},{"id":"W2805926240","doi":"10.3847/1538-4357/aac8da","title":"Dense Gas Kinematics and a Narrow Filament in the Orion A OMC1 Region Using NH<sub>3</sub>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Protein filament; Magnetic field; Turbulence; Orientation (vector space); Green Bank Telescope; Solar prominence; Orion Nebula; Angular resolution (graph drawing)","score_opus":0.019675110626850224,"score_gpt":0.24935175850374172,"score_spread":0.2296766478768915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2805926240","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988091,0.0000489139,0.00024163398,0.000031716165,0.0000013072672,0.0000031402656,0.00015283051,0.000047715785,0.00066363026],"genre_scores_gemma":[0.9990988,0.000020627182,0.00052438816,0.000010568572,0.000004007401,0.0000024223364,0.00023233614,0.00000997296,0.00009678203],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993324,0.0000064928377,0.000002100781,0.000022768116,0.000015950498,0.000019314242],"domain_scores_gemma":[0.99975985,0.000040356168,0.00009487024,0.00002380687,0.000021378983,0.00005982901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014444486,0.00021573376,0.00017484867,0.0006139703,0.0004933679,0.0004032854,0.00029170333,0.00025968062,0.0011174786],"category_scores_gemma":[0.0002115904,0.00015598994,0.00018693185,0.00040399688,0.00016062819,0.00016067446,0.0003223025,0.00021418386,0.00015391497],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005389521,0.00017998282,0.7169054,0.000061030667,0.00011732956,0.0010493904,0.0008880304,0.005820781,0.24986883,0.0004889615,0.000653194,0.023428101],"study_design_scores_gemma":[0.000012906202,0.000049756967,0.9858602,0.000011329635,0.000029714301,0.00012957292,0.00014086928,0.0071611446,0.0053796936,0.00013485883,0.0010802394,0.00000953798],"about_ca_topic_score_codex":0.010795749,"about_ca_topic_score_gemma":0.012233787,"teacher_disagreement_score":0.010795749,"about_ca_system_score_codex":0.0004515669,"about_ca_system_score_gemma":0.00015541937,"threshold_uncertainty_score":0.021465778},"labels":[],"label_agreement":null},{"id":"W2806511830","doi":"10.3847/1538-4357/aace62","title":"Variability Timescale and Spectral Index of Sgr A* in the Near Infrared: Approximate Bayesian Computation Analysis of the Variability of the Closest Supermassive Black Hole","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Spectral index; Supermassive black hole; Dimensionless quantity; Spectral density; Light curve; Accretion (finance); Milky Way; Computation","score_opus":0.007374717108367364,"score_gpt":0.2297329037370142,"score_spread":0.22235818662864681,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2806511830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91925037,0.00014485094,0.079192236,0.00016305066,0.0000060176617,0.000014541584,0.00028967825,0.00010389761,0.00083538913],"genre_scores_gemma":[0.9897943,0.000041668212,0.009502477,0.000016314425,0.000011075863,0.000012275235,0.00042049383,0.00001397639,0.00018738655],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99946755,0.00024117861,0.000029060206,0.00013595361,0.00009097581,0.000035192443],"domain_scores_gemma":[0.99684995,0.002318959,0.00034927655,0.00015217636,0.000237808,0.000091870366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017485189,0.00024432596,0.00042027843,0.00082027516,0.0003771006,0.0008263104,0.00043619613,0.00039769392,0.0005675674],"category_scores_gemma":[0.0073513915,0.0002526375,0.000580649,0.000495574,0.00038982357,0.0006401614,0.00045845666,0.00044984877,0.0001240924],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004491875,0.00011893308,0.21073934,0.00005447138,0.00035435008,0.0001335349,0.00024267231,0.71701735,0.0074156765,0.005974531,0.0006937236,0.056806237],"study_design_scores_gemma":[0.000005813229,0.000021434322,0.033185817,0.0000051125644,0.0000155949,0.000019882047,0.00002107828,0.96474755,0.00034097125,0.001510774,0.00011514712,0.000010789804],"about_ca_topic_score_codex":0.013187504,"about_ca_topic_score_gemma":0.007897198,"teacher_disagreement_score":0.013187504,"about_ca_system_score_codex":0.0005774141,"about_ca_system_score_gemma":0.00048028008,"threshold_uncertainty_score":0.026221454},"labels":[],"label_agreement":null},{"id":"W2806711606","doi":"10.3847/1538-4357/aaee73","title":"The 2016 Outburst of PSR J1119-6127: Cooling and a Spin-down-dominated Glitch","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Glitch; Pulsar; Magnetar; Black-body radiation; Millisecond pulsar; RADIUS; Flux (metallurgy); Neutron star","score_opus":0.009220160393948424,"score_gpt":0.3172445110964614,"score_spread":0.308024350702513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2806711606","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99841356,0.00008466291,0.0001323094,0.000085191714,0.00003322395,0.000012835105,0.0002287495,0.000029410685,0.0009800476],"genre_scores_gemma":[0.99868864,0.00007766075,0.000102653656,0.00006120314,0.000041442338,0.0000072473877,0.00058534875,0.000012002052,0.00042377802],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998915,0.000007884107,0.000009047814,0.00002583615,0.00003397413,0.000031660187],"domain_scores_gemma":[0.99952424,0.000026322488,0.00015673411,0.00005379603,0.000066591674,0.0001723924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026563773,0.000338276,0.0005247897,0.00037049677,0.00071070733,0.00056614785,0.000259221,0.00032369312,0.000988015],"category_scores_gemma":[0.00061499106,0.00015539567,0.00023723434,0.00032692382,0.00047761545,0.00021753342,0.000817641,0.00085395813,0.00043334987],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011903936,0.00030566473,0.84370875,0.00013861935,0.0001895533,0.008285307,0.0012795788,0.00088623655,0.123726144,0.00046189618,0.0032872364,0.01654075],"study_design_scores_gemma":[0.000021201915,0.00025286095,0.9928316,0.000013856926,0.00002315748,0.0008535857,0.00033214246,0.00049566163,0.0024774258,0.00010221399,0.0025843906,0.000011973177],"about_ca_topic_score_codex":0.0042175762,"about_ca_topic_score_gemma":0.0075871083,"teacher_disagreement_score":0.0042175762,"about_ca_system_score_codex":0.00042522233,"about_ca_system_score_gemma":0.00028974563,"threshold_uncertainty_score":0.008386016},"labels":[],"label_agreement":null},{"id":"W2806800495","doi":"10.3847/1538-4357/aac015","title":"Preferential Accretion in the Supermassive Black Holes of Milky Way-size Galaxies Due to Direct Feeding by Satellites","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Supermassive black hole; Astrophysics; Galaxy merger; Galaxy; Accretion (finance); Astronomy; Galaxy formation and evolution; Milky Way","score_opus":0.008879947962554568,"score_gpt":0.220269713368781,"score_spread":0.21138976540622645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2806800495","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995413,0.000040918676,0.00017288912,0.00001912131,0.0000018104234,0.0000016395761,0.000029964334,0.000013523809,0.00017894272],"genre_scores_gemma":[0.99974304,0.000019200352,0.000117136755,0.000007676058,0.0000020344419,0.0000011773031,0.000033578428,0.0000036766683,0.00007243325],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999199,0.000018597722,0.0000051841694,0.000018749915,0.000012122538,0.000025510779],"domain_scores_gemma":[0.99952936,0.0001029322,0.00017408805,0.000042071493,0.00003115413,0.00012049416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024818373,0.00031105502,0.00032596683,0.00055144937,0.00038183318,0.0007863198,0.00059868273,0.0004488441,0.001092509],"category_scores_gemma":[0.0011272035,0.00026117513,0.0007126909,0.0003098306,0.0004984216,0.00042867733,0.00085883227,0.0003023014,0.00009522576],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045073417,0.00024596264,0.7288944,0.00007116639,0.0005680135,0.001894092,0.00034294775,0.23181242,0.029049348,0.0024713983,0.00039055495,0.0038088993],"study_design_scores_gemma":[0.00013505603,0.00023849122,0.4487199,0.000014302487,0.00017079346,0.0003892139,0.00026826462,0.5454095,0.0032632598,0.0008654999,0.0004882423,0.000037462243],"about_ca_topic_score_codex":0.013130475,"about_ca_topic_score_gemma":0.007152568,"teacher_disagreement_score":0.013130475,"about_ca_system_score_codex":0.00066415704,"about_ca_system_score_gemma":0.00033911405,"threshold_uncertainty_score":0.026108146},"labels":[],"label_agreement":null},{"id":"W2807057946","doi":"10.3847/1538-4357/aac9b9","title":"The MAVERIC Survey: Still No Evidence for Accreting Intermediate-mass Black Holes in Globular Clusters","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Jansky; Accretion (finance); Black hole (networking); Telescope; Cluster (spacecraft); Star cluster; Galaxy cluster","score_opus":0.03599889225354671,"score_gpt":0.29085026378958734,"score_spread":0.25485137153604065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2807057946","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985863,0.00019126017,0.000038605693,0.000024434396,0.0000027216365,0.0000027770766,0.0002818357,0.0000065512327,0.0008655936],"genre_scores_gemma":[0.9988839,0.00008838207,0.00007425566,0.00003753631,0.000006808745,0.0000015874384,0.00067479303,0.000003510733,0.00022937184],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996449,0.00004956138,0.000022572534,0.0001137099,0.00007498111,0.00009431072],"domain_scores_gemma":[0.99846894,0.00016174445,0.00029326876,0.00025773392,0.00030867834,0.0005096099],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048291808,0.00017175307,0.0002804991,0.0014904034,0.0003967913,0.0008326878,0.00038665344,0.00022479692,0.001000553],"category_scores_gemma":[0.0011265321,0.00008397682,0.00013193261,0.000955751,0.00044822975,0.00032721693,0.0009123547,0.0001639003,0.00023248348],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045115183,0.0000103059765,0.99341255,0.000009865915,0.00003132643,0.000056407964,0.0002217517,0.000037113496,0.0028686365,0.0000818362,0.00023037691,0.0029947348],"study_design_scores_gemma":[0.0000021367389,0.000016208152,0.99908185,0.0000038699163,0.000010767312,0.000058498477,0.00017456611,0.000027902859,0.00013584516,0.000012889109,0.00047429206,0.0000011017129],"about_ca_topic_score_codex":0.0126679605,"about_ca_topic_score_gemma":0.033842046,"teacher_disagreement_score":0.0126679605,"about_ca_system_score_codex":0.00028651897,"about_ca_system_score_gemma":0.00035703243,"threshold_uncertainty_score":0.025188446},"labels":[],"label_agreement":null},{"id":"W2807730752","doi":"10.3847/1538-4357/aac168","title":"A MegaCam Survey of Outer Halo Satellites. I. Description of the Survey*<sup>†</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Globular cluster; Halo; Limiting; Galactic halo; Telescope; Stellar density; Dwarf galaxy","score_opus":0.021282952226261493,"score_gpt":0.2259313045435491,"score_spread":0.2046483523172876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2807730752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5775839,0.0037475147,0.009576365,0.0005295213,0.00009714696,0.0012953065,0.35346192,0.0013347516,0.05237355],"genre_scores_gemma":[0.4673418,0.0022819196,0.058561057,0.0008385147,0.00021298508,0.0011949751,0.44905543,0.00037215996,0.020141033],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998229,0.000016856602,0.000017612376,0.00003770002,0.00007602486,0.00002882858],"domain_scores_gemma":[0.9993686,0.00004300288,0.00012243255,0.00012661738,0.00016899641,0.00017021681],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033808913,0.00022963081,0.0001641806,0.0019661917,0.0002507513,0.00053517445,0.00051441864,0.00014644064,0.005214513],"category_scores_gemma":[0.0005772127,0.00019757044,0.00017591055,0.0028500776,0.00013344127,0.00030899904,0.0005963174,0.00020161607,0.002940118],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002499573,0.000113755894,0.6531992,0.00059555646,0.00008890965,0.00028425158,0.00060770975,0.00094637374,0.022764387,0.0029335206,0.07620467,0.24201174],"study_design_scores_gemma":[0.000024323912,0.000056921115,0.8673113,0.000066142835,0.000025401378,0.00029336783,0.00016314836,0.0007677172,0.0027416581,0.00025198763,0.12828639,0.000011610659],"about_ca_topic_score_codex":0.012236088,"about_ca_topic_score_gemma":0.02732815,"teacher_disagreement_score":0.012236088,"about_ca_system_score_codex":0.00042765692,"about_ca_system_score_gemma":0.0006786327,"threshold_uncertainty_score":0.024329722},"labels":[],"label_agreement":null},{"id":"W2807808701","doi":"10.3847/1538-4357/aacbd0","title":"HESS J1943+213: An Extreme Blazar Shining through the Galactic Plane","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Blazar; Spectral energy distribution; Galactic plane; Polarization (electrochemistry); Very-long-baseline interferometry; Flux (metallurgy); BL Lac object; Very Long Baseline Array; Synchrotron; Synchrotron radiation","score_opus":0.026504230472399512,"score_gpt":0.2536034907751892,"score_spread":0.22709926030278965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2807808701","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977137,0.00003881058,0.00012127376,0.000040027593,0.000003818194,0.0000051349534,0.00046696892,0.0000484031,0.0015618806],"genre_scores_gemma":[0.99912554,0.000015833444,0.00016282663,0.000014774941,0.0000048991565,0.000001527326,0.00039265832,0.00000579918,0.0002762259],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996567,0.0000023698394,0.000001702243,0.00001103376,0.000008533998,0.000010634384],"domain_scores_gemma":[0.99991536,0.000009164897,0.00003015659,0.00001320454,0.0000059753256,0.000026118349],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000061573985,0.00020454923,0.00020511051,0.00040446722,0.00034034628,0.00035596473,0.00019556895,0.00027609288,0.0022818847],"category_scores_gemma":[0.00012947172,0.00009422619,0.00018321349,0.0005174278,0.00016419627,0.00011282159,0.00024033034,0.00017837077,0.00043793538],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006329737,0.00015699863,0.8713061,0.000060428356,0.00014123821,0.0087146675,0.0003719391,0.003313548,0.09312653,0.0008883193,0.003579263,0.017707942],"study_design_scores_gemma":[0.000019726156,0.00009399826,0.9919452,0.000006628578,0.000020753112,0.001259763,0.00012020107,0.001815865,0.0021327995,0.00019967658,0.0023758267,0.000009479925],"about_ca_topic_score_codex":0.0059178537,"about_ca_topic_score_gemma":0.00900567,"teacher_disagreement_score":0.0059178537,"about_ca_system_score_codex":0.00040279017,"about_ca_system_score_gemma":0.00008590213,"threshold_uncertainty_score":0.011766791},"labels":[],"label_agreement":null},{"id":"W2807813916","doi":"10.3847/1538-4357/aacb81","title":"The Globular Cluster Systems of Ultra-diffuse Galaxies in the Coma Cluster","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Coma Cluster; Globular cluster; Galaxy; Stellar density; Star cluster; Stellar mass; Dwarf spheroidal galaxy; Dwarf galaxy","score_opus":0.007416455498406086,"score_gpt":0.21574455367052658,"score_spread":0.2083280981721205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2807813916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994123,0.00006750724,0.0000227992,0.000006669183,5.5419946e-7,0.0000012535471,0.000083574196,0.00000259714,0.00040273718],"genre_scores_gemma":[0.9997422,0.000019666497,0.000024971892,0.0000032324613,7.298695e-7,4.785113e-7,0.0001225356,5.439822e-7,0.000085539876],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998485,0.000018321114,0.000007338156,0.000044669436,0.000027219403,0.000053989956],"domain_scores_gemma":[0.9996604,0.000027928736,0.00010814512,0.000029525221,0.000049385497,0.00012480674],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016383483,0.00015629634,0.000121673496,0.0013228259,0.0005296039,0.00050878053,0.00017840191,0.000115714036,0.00110112],"category_scores_gemma":[0.00041956268,0.00010815017,0.000101291684,0.0008705972,0.00046197145,0.00025212637,0.00066867366,0.000098701144,0.00014451126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000044096523,0.0000070048986,0.99576086,0.000005677621,0.000023434814,0.00008404023,0.000308639,0.000071887596,0.0016153862,0.00010899182,0.00010093554,0.0018691581],"study_design_scores_gemma":[5.884961e-7,0.0000048419984,0.999592,9.437554e-7,0.0000024419578,0.000044191314,0.00011144203,0.000052955034,0.000057253565,0.000020415127,0.00011195793,9.5334696e-7],"about_ca_topic_score_codex":0.026682714,"about_ca_topic_score_gemma":0.044268362,"teacher_disagreement_score":0.026682714,"about_ca_system_score_codex":0.00063442806,"about_ca_system_score_gemma":0.00021387554,"threshold_uncertainty_score":0.05305481},"labels":[],"label_agreement":null},{"id":"W2807897321","doi":"10.3847/1538-4357/ab06f8","title":"Mass and Mass Scalings of Super-Earths","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Photoevaporation; Planet; Planetary mass; RADIUS; Planetary migration; Population; Planetary system; Radial velocity; Metallicity; Exoplanet","score_opus":0.006519411178218037,"score_gpt":0.20362779062983047,"score_spread":0.19710837945161244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2807897321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99639016,0.0001595274,0.0007632618,0.00002054293,0.0000032923745,0.0000026885573,0.00009306402,0.000036502064,0.0025309008],"genre_scores_gemma":[0.9995648,0.00002691436,0.00017035597,0.000003406653,0.0000035860703,0.0000010323796,0.00006280532,0.000007121544,0.0001599469],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998859,0.000008877656,0.0000038295734,0.000059045826,0.000020169326,0.000022224207],"domain_scores_gemma":[0.9993412,0.00018045267,0.00022227132,0.00009187818,0.00006992617,0.00009417819],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001692861,0.00014263735,0.00014394904,0.0010699149,0.00016879964,0.0004395313,0.00022908761,0.00025146932,0.0019327289],"category_scores_gemma":[0.0011320297,0.00013749932,0.00012776478,0.00029842954,0.00032967402,0.00072590413,0.0005405193,0.00020049157,0.00036578928],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053752307,0.00006454796,0.78595006,0.000103625745,0.0001539511,0.00093646324,0.0014274777,0.012964651,0.14341438,0.01350862,0.00072489976,0.040213704],"study_design_scores_gemma":[0.000016640633,0.00014357285,0.94372785,0.000015863952,0.000031929532,0.00086966425,0.000335031,0.021321367,0.02327934,0.0054803267,0.0047560125,0.000022443946],"about_ca_topic_score_codex":0.000339997,"about_ca_topic_score_gemma":0.00021309267,"teacher_disagreement_score":0.0019327289,"about_ca_system_score_codex":0.00020941014,"about_ca_system_score_gemma":0.000030923606,"threshold_uncertainty_score":0.0064656734},"labels":[],"label_agreement":null},{"id":"W2808001639","doi":"10.3847/1538-4357/aac16b","title":"A MegaCam Survey of Outer Halo Satellites. III. Photometric and Structural Parameters*<sup>†</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":189,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Halo; Globular cluster; Surface brightness; Galactic halo; Galaxy; Telescope","score_opus":0.019094425786838794,"score_gpt":0.245080848587536,"score_spread":0.22598642280069722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2808001639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99524397,0.00022920304,0.00026857105,0.000017379298,0.0000012635697,0.000009340381,0.0030631558,0.00002778939,0.0011392884],"genre_scores_gemma":[0.98801893,0.00016797871,0.0016714776,0.000023977233,0.0000089714795,0.000014844532,0.009521109,0.000016818398,0.000555767],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989057,0.00001550013,0.000008822701,0.000024023497,0.000040567786,0.000020574993],"domain_scores_gemma":[0.99928504,0.0000902184,0.00021804127,0.00010174907,0.00017250852,0.00013252003],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031982563,0.00014935056,0.00013877382,0.0015816219,0.00016562088,0.00033199886,0.00027193027,0.000110634806,0.00097474793],"category_scores_gemma":[0.0007759697,0.00012754567,0.00018521887,0.001561225,0.00013900557,0.00022983913,0.00051721674,0.00011781714,0.000459207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005532679,0.00001335269,0.97989583,0.000028185032,0.000034613837,0.00004539423,0.00017701296,0.00034067745,0.0027462004,0.00013474477,0.0008578895,0.015670873],"study_design_scores_gemma":[0.0000034074162,0.000010058592,0.9976173,0.0000043864184,0.0000090918,0.000058458703,0.00006672922,0.00043756893,0.00045979948,0.000026536518,0.0013045991,0.0000020596171],"about_ca_topic_score_codex":0.008548852,"about_ca_topic_score_gemma":0.018120708,"teacher_disagreement_score":0.008548852,"about_ca_system_score_codex":0.00027314606,"about_ca_system_score_gemma":0.00016604006,"threshold_uncertainty_score":0.016998172},"labels":[],"label_agreement":null},{"id":"W2808482821","doi":"10.3847/1538-4357/aad084","title":"Binary Pulsar Distances and Velocities from Gaia Data Release 2","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Australian Research Council; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Durham University; Smithsonian Institution","keywords":"Pulsar; Physics; Parallax; Millisecond pulsar; Astrometry; Astrophysics; Proper motion; Astronomy; White dwarf; Binary number; Photometry (optics); Binary pulsar; Stars","score_opus":0.023691633126791095,"score_gpt":0.32753906239546793,"score_spread":0.3038474292686768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2808482821","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47525603,0.0004861939,0.0015076098,0.00015848322,0.000083849096,0.00014163325,0.5053588,0.0019859555,0.015021463],"genre_scores_gemma":[0.27109757,0.00010462075,0.0027615272,0.0000896543,0.000044839784,0.00019360009,0.72335154,0.00026273474,0.0020938993],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993594,0.00004632089,0.00008496339,0.00018372037,0.00021086096,0.00011476279],"domain_scores_gemma":[0.9974285,0.0001761453,0.00089340407,0.00049073936,0.0007746004,0.0002365949],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065048574,0.00067915546,0.00053440547,0.0055419225,0.0003399944,0.00124472,0.0006605781,0.00043523088,0.0028579552],"category_scores_gemma":[0.0028367324,0.0002727328,0.000549459,0.004272622,0.00013632176,0.00054993556,0.0011045218,0.00055211096,0.0041768],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013420557,0.00022968605,0.8271207,0.00044071864,0.0006683528,0.00042184658,0.00045613854,0.008116437,0.01029982,0.0013622718,0.10207771,0.047464214],"study_design_scores_gemma":[0.00010265108,0.00007999607,0.9447198,0.000040518542,0.00007315937,0.00016645207,0.0000981439,0.0036244416,0.0020987215,0.00017982765,0.048778288,0.000038094408],"about_ca_topic_score_codex":0.027176954,"about_ca_topic_score_gemma":0.018433504,"teacher_disagreement_score":0.027176954,"about_ca_system_score_codex":0.0006663193,"about_ca_system_score_gemma":0.000541495,"threshold_uncertainty_score":0.05403751},"labels":[],"label_agreement":null},{"id":"W2808486150","doi":"10.3847/1538-4357/aacbca","title":"Comparison of the Extraplanar Hα and UV Emissions in the Halos of Nearby Edge-on Spiral Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy; Spiral galaxy; Disc; Luminous infrared galaxy; Scale height; Star formation; Scale (ratio); Emission spectrum","score_opus":0.016784015381679424,"score_gpt":0.26281348596171206,"score_spread":0.24602947058003263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2808486150","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994867,0.0000459696,0.00004455459,0.0000028870365,4.1223586e-7,7.79012e-7,0.000052483916,0.0000033906122,0.00036295084],"genre_scores_gemma":[0.99964297,0.000032756132,0.000050936873,0.0000033530796,0.0000013576224,6.987468e-7,0.00016226328,0.0000014351663,0.00010430031],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999931,0.000007825881,0.0000034715413,0.000017350276,0.00001409145,0.00002635654],"domain_scores_gemma":[0.9995869,0.000063433945,0.00011513031,0.00003376716,0.00005978592,0.00014095813],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109754474,0.00022451546,0.00013396614,0.0012798072,0.00017140932,0.00039543494,0.00012337892,0.00013516241,0.001038275],"category_scores_gemma":[0.00043142648,0.00011269406,0.00014053585,0.00048589747,0.0002515885,0.00016308141,0.0004046637,0.00008070593,0.00015647335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015279002,0.00001762626,0.9696332,0.000013225553,0.000050557355,0.00015936099,0.00033277224,0.00017413394,0.02512259,0.0000722122,0.00004213989,0.004229345],"study_design_scores_gemma":[0.0000014855583,0.000020728134,0.9992029,0.0000020912642,0.000004659142,0.000071929935,0.000098432894,0.00007449453,0.00040665502,0.00002063974,0.00009478666,0.0000011250784],"about_ca_topic_score_codex":0.0042985673,"about_ca_topic_score_gemma":0.007062842,"teacher_disagreement_score":0.0042985673,"about_ca_system_score_codex":0.00019897982,"about_ca_system_score_gemma":0.000059476723,"threshold_uncertainty_score":0.008547068},"labels":[],"label_agreement":null},{"id":"W2808606823","doi":"10.3847/1538-4357/aacce2","title":"Effect of the Heating Rate on the Stability of the Three-phase Interstellar Medium","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of British Columbia","funders":"","keywords":"Physics; Interstellar medium; Astrophysics; Phase (matter); Astronomy; Interstellar cloud; Astrochemistry; Astrobiology; Galaxy","score_opus":0.012760143350314564,"score_gpt":0.2664140931970104,"score_spread":0.25365394984669587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2808606823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9920167,0.000145662,0.0012041626,0.0002680095,0.000028876153,0.000022227745,0.0002561541,0.00012895772,0.0059292754],"genre_scores_gemma":[0.9988458,0.000056698576,0.00051411876,0.000038563576,0.000005478661,0.000013306731,0.000103300445,0.000041216455,0.00038153632],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999876,0.000022820244,0.0000048565794,0.000018481296,0.000027607337,0.000050166465],"domain_scores_gemma":[0.9992155,0.00042563555,0.000095827825,0.00006439813,0.000096382704,0.000102357066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036439774,0.00047729554,0.0004314242,0.00035160378,0.0006802713,0.0010452903,0.0005995316,0.0006366622,0.0023679652],"category_scores_gemma":[0.0020496666,0.00030276578,0.00061569276,0.00029555729,0.00094522454,0.00059880543,0.0006103538,0.0010024704,0.00022623218],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082936103,0.00025044853,0.015427497,0.00011726316,0.00016425255,0.00055712427,0.0002097559,0.9179513,0.050533306,0.008605833,0.001227135,0.004126781],"study_design_scores_gemma":[0.0001544451,0.0001868791,0.007787591,0.000021476968,0.000054663837,0.00005024145,0.00014682079,0.971193,0.018051468,0.0016759868,0.00062678044,0.00005064912],"about_ca_topic_score_codex":0.010606201,"about_ca_topic_score_gemma":0.0035529868,"teacher_disagreement_score":0.010606201,"about_ca_system_score_codex":0.000939566,"about_ca_system_score_gemma":0.0007182005,"threshold_uncertainty_score":0.021088958},"labels":[],"label_agreement":null},{"id":"W2808618292","doi":"10.3847/1538-4357/aaccfc","title":"Spiral Arms in Disks: Planets or Gravitational Instability?","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Planet; Astrophysics; Stars; Astronomy; Spiral galaxy; Accretion (finance); Gravitational instability; Planetary system; Protoplanetary disk; Giant planet; Galaxy","score_opus":0.01737859203819674,"score_gpt":0.271122719842762,"score_spread":0.25374412780456523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2808618292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9792255,0.013607377,0.001172252,0.0015640509,0.000049048496,0.00000583177,0.00012223437,0.00003695031,0.0042166975],"genre_scores_gemma":[0.99845064,0.0010400595,0.0001242351,0.00006249627,0.000056829904,9.07252e-7,0.000024279567,0.0000017952269,0.00023872155],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998652,0.000027525803,0.000012046563,0.000038237267,0.000024204233,0.000032861237],"domain_scores_gemma":[0.99841034,0.00055935624,0.00059826905,0.00010979559,0.00014490102,0.00017736688],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046559836,0.00014932237,0.00024241768,0.0012004428,0.00030854862,0.0010530972,0.00033032085,0.00069378456,0.0028657357],"category_scores_gemma":[0.002156012,0.000087520195,0.00008040819,0.00094636495,0.0011221798,0.001239682,0.00036626623,0.00018299455,0.00035079962],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003334907,0.000051759915,0.8979258,0.00030981758,0.00006593076,0.0020655757,0.0023554196,0.0005272459,0.017173646,0.009604134,0.0016935449,0.067893624],"study_design_scores_gemma":[0.000021492478,0.00016417765,0.94742864,0.00023056536,0.000046213092,0.010338166,0.0036215438,0.0016729247,0.0021912798,0.020079335,0.014177417,0.000028363851],"about_ca_topic_score_codex":0.0011056093,"about_ca_topic_score_gemma":0.0008635054,"teacher_disagreement_score":0.0028657357,"about_ca_system_score_codex":0.00027708942,"about_ca_system_score_gemma":0.00009770245,"threshold_uncertainty_score":0.009586811},"labels":[],"label_agreement":null},{"id":"W2808763289","doi":"10.3847/1538-4357/aacdaa","title":"A Machine-learning Method for Identifying Multiwavelength Counterparts of Submillimeter Galaxies: Training and Testing Using AS2UDS and ALESS","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of British Columbia","funders":"National Institutes of Natural Sciences; National Key Research and Development Program of China; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Korea Astronomy and Space Science Institute; China Scholarship Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Durham University; National Science Council; National Natural Science Foundation of China; National Radio Astronomy Observatory; Narodowym Centrum Nauki; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Photometric redshift; Redshift; Luminous infrared galaxy; Submillimeter Array; Astronomy; Star formation","score_opus":0.04502542102455129,"score_gpt":0.295049873724407,"score_spread":0.25002445269985574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2808763289","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8243888,0.00040279527,0.16194424,0.00025590995,0.00009001825,0.00015852181,0.0016168692,0.00828042,0.0028623692],"genre_scores_gemma":[0.88582474,0.000050070714,0.10813223,0.00012916775,0.000042839638,0.0001630378,0.0040273354,0.00014575836,0.0014846687],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99871063,0.0005452597,0.00007203918,0.0003481088,0.00020575199,0.000118225216],"domain_scores_gemma":[0.9967159,0.0015122499,0.00027778454,0.0007015925,0.0006267865,0.00016575588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003143051,0.0011087725,0.0007509553,0.0022475573,0.00064897386,0.00072237675,0.0018209665,0.0011931725,0.0017330016],"category_scores_gemma":[0.0054865787,0.0003470277,0.00078201934,0.0009841748,0.00055481243,0.0006430541,0.0009954609,0.00093641266,0.0010120282],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000746333,0.0010939711,0.20822392,0.00015615638,0.0005590389,0.0004386181,0.00020885274,0.3024982,0.014655535,0.0014602878,0.011526863,0.45843226],"study_design_scores_gemma":[0.000019054014,0.00004222604,0.006837805,0.0000070635533,0.000015846743,0.00002507509,0.000029270916,0.9888249,0.0030562023,0.0005166117,0.00061929924,0.000006602429],"about_ca_topic_score_codex":0.00763961,"about_ca_topic_score_gemma":0.0076961606,"teacher_disagreement_score":0.00763961,"about_ca_system_score_codex":0.0004825888,"about_ca_system_score_gemma":0.0006434813,"threshold_uncertainty_score":0.016622245},"labels":[],"label_agreement":null},{"id":"W2809742465","doi":"10.3847/1538-4357/aacaff","title":"Erratum: “CHANG-ES. V. Nuclear Outflow in a Virgo Cluster Spiral after a Tidal Disruption Event” (2015, ApJ, 809, 172)","year":2018,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Virgo Cluster; Outflow; Astrophysics; Spiral (railway); Event (particle physics); Cluster (spacecraft); Astronomy; Galaxy; Meteorology; Galaxy cluster","score_opus":0.006878585243762306,"score_gpt":0.23397152355745657,"score_spread":0.22709293831369426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2809742465","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0009442161,0.0009607459,0.00028835275,0.05014075,0.9404638,0.000020597785,0.0011076641,0.00029598718,0.005777883],"genre_scores_gemma":[0.035330705,0.009259357,0.00307308,0.15023763,0.38706112,0.00014806447,0.007651022,0.0014393767,0.40579966],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9990797,0.00008999261,0.00020843446,0.00017375204,0.00034271067,0.000105355095],"domain_scores_gemma":[0.9959888,0.00090926234,0.00039167205,0.00027331617,0.002084765,0.0003521512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010797988,0.0017041068,0.0011201954,0.0022186611,0.0033726864,0.002193858,0.002112587,0.005136425,0.027530823],"category_scores_gemma":[0.012217164,0.0005979893,0.0010003486,0.0014025464,0.0015543225,0.0019045206,0.0016048446,0.006067421,0.022354368],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000604114,0.0000108860095,0.00019978538,0.00006654538,0.000007799062,0.00057713257,0.000034297776,0.0000410052,0.00009705964,0.000494297,0.99486524,0.003545488],"study_design_scores_gemma":[0.000045230718,0.00004829598,0.003399857,0.00025154228,0.00004104463,0.00095704,0.00019913497,0.0002167659,0.000554503,0.001383711,0.99285275,0.00005021882],"about_ca_topic_score_codex":0.019555928,"about_ca_topic_score_gemma":0.020518279,"teacher_disagreement_score":0.027530823,"about_ca_system_score_codex":0.0025753886,"about_ca_system_score_gemma":0.0025567976,"threshold_uncertainty_score":0.092099786},"labels":[],"label_agreement":null},{"id":"W2810004840","doi":"10.3847/1538-4357/aacf9e","title":"On the Sensitivity of Magnetic Cycles in Global Simulations of Solar-like Stars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Dynamo; Rossby number; Dynamo theory; Differential rotation; Convection; Magnetic field; Equator; Magnetohydrodynamics","score_opus":0.007434947443978587,"score_gpt":0.238735838556594,"score_spread":0.23130089111261543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2810004840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928247,0.000087716275,0.0017450546,0.00022462456,0.00002930482,0.000026485155,0.0003764556,0.00011685497,0.004568785],"genre_scores_gemma":[0.99842143,0.00003901307,0.00092059124,0.00005720065,0.0000065914087,0.000021297385,0.0002609954,0.00003270263,0.0002401586],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998004,0.00007997997,0.000013495024,0.000032067543,0.000029564073,0.000044513137],"domain_scores_gemma":[0.99792767,0.0013678446,0.00018196563,0.00015049026,0.00018882117,0.0001831392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00084057456,0.0005475615,0.00064050406,0.00052961573,0.0006552743,0.001014683,0.0006602816,0.0010166619,0.0021019941],"category_scores_gemma":[0.0048554908,0.0003029422,0.0005406943,0.00046941638,0.00088281493,0.0005954309,0.0007980023,0.00086583,0.00014032454],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015929069,0.00016994274,0.020413613,0.000039711365,0.000088557055,0.00008722893,0.00008222346,0.9737814,0.0014925944,0.0015341046,0.00045755782,0.0016937766],"study_design_scores_gemma":[0.00003689579,0.000061859806,0.003130893,0.000009238314,0.000011332878,0.000008587896,0.00006260928,0.9953784,0.00045424205,0.0005820437,0.00025615247,0.000007762306],"about_ca_topic_score_codex":0.013940129,"about_ca_topic_score_gemma":0.007261207,"teacher_disagreement_score":0.013940129,"about_ca_system_score_codex":0.00073416554,"about_ca_system_score_gemma":0.0005558891,"threshold_uncertainty_score":0.027717948},"labels":[],"label_agreement":null},{"id":"W2810239085","doi":"10.3847/1538-4357/aac9c9","title":"The NANOGrav 11 yr Data Set: Arecibo Observatory Polarimetry and Pulse Microcomponents","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"","keywords":"Pulsar; Polarimetry; Observatory; Millisecond pulsar; Polarization (electrochemistry); Pulse (music); Gravitational wave","score_opus":0.037270122565047706,"score_gpt":0.34014713833564036,"score_spread":0.3028770157705927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2810239085","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.66557854,0.00058166805,0.0020404453,0.00026153054,0.00011050468,0.00013941046,0.3095501,0.000761582,0.020976167],"genre_scores_gemma":[0.33958283,0.0003414782,0.003725885,0.0001406933,0.000088369576,0.00024777267,0.6513052,0.00021043782,0.0043572783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996693,0.000029126424,0.000024058734,0.00008889062,0.00012997708,0.000058571124],"domain_scores_gemma":[0.9988438,0.00012185214,0.00032940423,0.00032947963,0.00028726243,0.000088214074],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046525433,0.00043731983,0.0004985651,0.0024580376,0.00046730263,0.00066171255,0.0005407154,0.00031765684,0.0048814295],"category_scores_gemma":[0.0011927583,0.0001658935,0.0002690866,0.0043012314,0.0001907926,0.00027995996,0.0007412681,0.00035386052,0.0026379682],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002760143,0.0005185851,0.7192564,0.00050743757,0.00053393905,0.0006189589,0.00036683274,0.0077653527,0.038107585,0.0014860553,0.10423551,0.12384324],"study_design_scores_gemma":[0.000117019816,0.000050078957,0.93691796,0.000024995328,0.000043275377,0.00013701306,0.00008082492,0.0022794292,0.002908715,0.0001436738,0.057275165,0.000021789589],"about_ca_topic_score_codex":0.02414052,"about_ca_topic_score_gemma":0.031644635,"teacher_disagreement_score":0.02414052,"about_ca_system_score_codex":0.00045686561,"about_ca_system_score_gemma":0.00047737604,"threshold_uncertainty_score":0.047999978},"labels":[],"label_agreement":null},{"id":"W2810325998","doi":"10.3847/1538-4357/aad09b","title":"The WFC3 Galactic Bulge Treasury Program: Relative Ages of Bulge Stars of High and Low Metallicity<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Bulge; Globular cluster; Milky Way; Stars; Galaxy; Metallicity; Photometry (optics); Luminosity","score_opus":0.011651746966256022,"score_gpt":0.27146891209081486,"score_spread":0.2598171651245588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2810325998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8540642,0.00036820924,0.0037663747,0.00018227383,0.000024683943,0.000060400307,0.13357683,0.0016222326,0.00633472],"genre_scores_gemma":[0.87301505,0.00010677648,0.006575364,0.00006417006,0.000022042834,0.00006856412,0.11854175,0.00038308537,0.0012231895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999828,0.0000135289265,0.000009340244,0.000040542156,0.00004122331,0.000067363304],"domain_scores_gemma":[0.9988914,0.00011164413,0.00033312826,0.00017921801,0.00024786984,0.0002366129],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068740913,0.00037011923,0.00028252386,0.0021407786,0.00049954554,0.0008245449,0.0005856209,0.00036989225,0.0041664853],"category_scores_gemma":[0.0008048448,0.000119971395,0.00048497226,0.002530943,0.00023232016,0.00040873434,0.000469753,0.00030555687,0.0024561922],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008739494,0.000057422098,0.91970354,0.00007887312,0.00018035911,0.00018585393,0.00030181775,0.0014624695,0.01592564,0.00047974227,0.0221739,0.038576365],"study_design_scores_gemma":[0.000007967176,0.0000119507085,0.9940456,0.0000059342474,0.00001657112,0.00005438651,0.00006959876,0.000939694,0.0022654145,0.000089327885,0.0024868527,0.0000066677853],"about_ca_topic_score_codex":0.04485864,"about_ca_topic_score_gemma":0.063122824,"teacher_disagreement_score":0.04485864,"about_ca_system_score_codex":0.0006177824,"about_ca_system_score_gemma":0.0003132023,"threshold_uncertainty_score":0.08919507},"labels":[],"label_agreement":null},{"id":"W2811044042","doi":"10.3847/0004-637x/829/1/21","title":"MULTI-WAVELENGTH LENS RECONSTRUCTION OF A PLANCK AND HERSCHEL-DETECTED STAR-BURSTING GALAXY","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Stars; Galaxy cluster; Lens (geology); Type-cD galaxy; Brightest cluster galaxy; Gravitational lens; Planck; Elliptical galaxy","score_opus":0.012365913056513012,"score_gpt":0.20734313706917398,"score_spread":0.19497722401266096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2811044042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9895,0.00016388022,0.0058779237,0.00013297828,0.000009195141,0.000008637936,0.0018551451,0.0005938647,0.0018584094],"genre_scores_gemma":[0.994083,0.000052370942,0.0045609367,0.000020484968,0.0000071180643,0.0000023636621,0.00083689974,0.000053647662,0.0003832494],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989533,0.000012312879,0.0000036513234,0.000033932425,0.000028889675,0.000025847687],"domain_scores_gemma":[0.9996376,0.00004656573,0.00010288426,0.000069653615,0.000059573067,0.00008371382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021742251,0.00042680698,0.00030099147,0.0012778388,0.00021406976,0.00059850933,0.0005150609,0.00045568086,0.003057135],"category_scores_gemma":[0.0005001554,0.000371949,0.0008754753,0.00083857414,0.00022539421,0.0003208903,0.000489627,0.00031145505,0.0006155431],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008384995,0.0001968898,0.43162492,0.00026300724,0.0009115052,0.0028269878,0.0006270102,0.3729843,0.13244684,0.0030400043,0.0033126506,0.050927363],"study_design_scores_gemma":[0.000035410638,0.00009891225,0.64096063,0.000024759398,0.00011076684,0.00068464346,0.00020629143,0.3434803,0.0111019565,0.0009195439,0.0022978298,0.000078949335],"about_ca_topic_score_codex":0.014423022,"about_ca_topic_score_gemma":0.014942276,"teacher_disagreement_score":0.014423022,"about_ca_system_score_codex":0.0012588929,"about_ca_system_score_gemma":0.00032587576,"threshold_uncertainty_score":0.02867812},"labels":[],"label_agreement":null},{"id":"W2811084038","doi":"10.3847/1538-4357/ab1a39","title":"Kinematics of Cluster Galaxies and Their Relation to Galaxy Evolution","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Astrophysics; Physics; Kinematics; Galaxy; Satellite galaxy; Brightest cluster galaxy; Galaxy cluster; Cluster (spacecraft); Galaxy formation and evolution; Satellite; Astronomy; Elliptical galaxy; Peculiar galaxy; Galaxy merger; Galaxy group; Classical mechanics; Computer science","score_opus":0.005502215007713816,"score_gpt":0.19888895431927325,"score_spread":0.19338673931155945,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2811084038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981383,0.000043648986,0.00087737915,0.000029235456,0.0000015877337,0.0000031510817,0.00006353198,0.000028525716,0.0008145789],"genre_scores_gemma":[0.9996562,0.000014095089,0.0001809646,0.0000023773764,6.421742e-7,9.032232e-7,0.000039201037,0.0000031131276,0.00010252162],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989784,0.00002790217,0.000003564291,0.000030512841,0.000018082777,0.000022099308],"domain_scores_gemma":[0.9991443,0.00026196794,0.0002381211,0.00011629236,0.00011622861,0.00012312089],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003006877,0.00022007085,0.00019271825,0.00054883456,0.00032739635,0.00091775064,0.0003645279,0.00029853536,0.0009660251],"category_scores_gemma":[0.002326746,0.00024285536,0.00021559474,0.00045945347,0.0005857261,0.0003669637,0.00043216962,0.00030173792,0.00018073818],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014661669,0.00005434273,0.7088157,0.00001776599,0.00010258508,0.00014002863,0.00033035871,0.2706226,0.00881721,0.0067597963,0.00025669872,0.0039363457],"study_design_scores_gemma":[0.000029085888,0.000104342216,0.6563133,0.000009592285,0.0000333129,0.0001159708,0.0002821414,0.334592,0.0040690424,0.0037085568,0.00070320466,0.00003940443],"about_ca_topic_score_codex":0.019724669,"about_ca_topic_score_gemma":0.009162308,"teacher_disagreement_score":0.019724669,"about_ca_system_score_codex":0.0010323274,"about_ca_system_score_gemma":0.0003189201,"threshold_uncertainty_score":0.039219737},"labels":[],"label_agreement":null},{"id":"W2811143277","doi":"10.3847/1538-4357/aad086","title":"Probing the Innermost Accretion Flow Geometry of Sgr A* with Event Horizon Telescope","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Perimeter Institute","funders":"","keywords":"Event horizon; Black hole (networking); Accretion (finance); Spin-flip; Radiative transfer; Flow (mathematics); Intermediate-mass black hole; Active galactic nucleus; Observable","score_opus":0.009752915245742119,"score_gpt":0.22642300681608268,"score_spread":0.21667009157034056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2811143277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9842678,0.00016077698,0.008821816,0.000075832766,0.000013439153,0.000025853164,0.00093709485,0.00032449298,0.005372996],"genre_scores_gemma":[0.9956736,0.000034736462,0.0035528908,0.000015661535,0.0000124530225,0.0000034329294,0.00043969753,0.000029811321,0.00023761504],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989915,0.00001615441,0.0000031281888,0.000033121105,0.00002011055,0.000028278857],"domain_scores_gemma":[0.99966633,0.000048119728,0.000117467716,0.000042035343,0.000036281723,0.00008982604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039241902,0.00027139,0.00021475255,0.00054681074,0.00027320153,0.00059979194,0.00035877476,0.00020135462,0.0014875308],"category_scores_gemma":[0.00046242392,0.0002006394,0.00040939866,0.00025995955,0.0003109637,0.00043605606,0.00041307995,0.00028667992,0.00019726307],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012026522,0.00025237276,0.34362227,0.00016563515,0.0002521449,0.0012809336,0.000662599,0.029342897,0.57095164,0.012028537,0.002452034,0.037786175],"study_design_scores_gemma":[0.00007237904,0.00021148512,0.8744371,0.000023548351,0.000058354137,0.0005045805,0.00014489805,0.10316025,0.016673515,0.00261128,0.002049185,0.000053448362],"about_ca_topic_score_codex":0.0037846016,"about_ca_topic_score_gemma":0.003269175,"teacher_disagreement_score":0.0037846016,"about_ca_system_score_codex":0.00057880435,"about_ca_system_score_gemma":0.00017376436,"threshold_uncertainty_score":0.007525146},"labels":[],"label_agreement":null},{"id":"W2811351113","doi":"10.3847/1538-4357/aacf04","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Quasar Host Galaxies at z &lt; 0.8 from Image Decomposition","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Quasar; Galaxy; Redshift; Photometry (optics); Sky; Luminosity; Astronomy; Active galactic nucleus; Stars","score_opus":0.010973990010549906,"score_gpt":0.2354426265339933,"score_spread":0.2244686365234434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2811351113","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84854084,0.00029461083,0.0033569077,0.00010284355,0.000012127081,0.000113005844,0.13982229,0.0011503819,0.006606967],"genre_scores_gemma":[0.59107137,0.00022033839,0.010829621,0.00004163535,0.000029640541,0.00016774374,0.39327314,0.00029877757,0.0040677623],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996629,0.000045179968,0.000020945716,0.00006192927,0.00012439638,0.00008463937],"domain_scores_gemma":[0.99911505,0.000045477915,0.00023714984,0.0001844362,0.0002829887,0.0001348798],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006421651,0.00048989983,0.00024716687,0.0037396476,0.00023950891,0.0007168828,0.0003499198,0.00015275522,0.0037628533],"category_scores_gemma":[0.00083783845,0.0001904687,0.000308606,0.0026747354,0.00010403402,0.0002495207,0.00080012094,0.00017109174,0.0020358155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005485999,0.00022848645,0.7421253,0.0002774115,0.0002745697,0.0004152162,0.0008928649,0.0043826746,0.025165694,0.00089938944,0.065591075,0.15919875],"study_design_scores_gemma":[0.000014395799,0.000018681374,0.98546946,0.000009638392,0.000018606203,0.00006405437,0.00007926114,0.0015896896,0.0016676281,0.000090171925,0.010972059,0.0000063580665],"about_ca_topic_score_codex":0.03357579,"about_ca_topic_score_gemma":0.03796619,"teacher_disagreement_score":0.03357579,"about_ca_system_score_codex":0.00041572275,"about_ca_system_score_gemma":0.0004894343,"threshold_uncertainty_score":0.06676066},"labels":[],"label_agreement":null},{"id":"W2813331457","doi":"10.3847/1538-4357/aad2e1","title":"Near-infrared High-resolution Imaging Polarimetry of FU Ori-type Objects: Toward a Unified Scheme for Low-mass Protostellar Evolution*","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Polarimetry; Stars; Young stellar object; Accretion (finance); Circumstellar dust; Polarization (electrochemistry); Reflection nebula; Nebula; Reflection (computer programming)","score_opus":0.010870281426379039,"score_gpt":0.24671380412927088,"score_spread":0.23584352270289183,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2813331457","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99263847,0.00037435134,0.0050217463,0.000039234466,0.000003739638,0.00001603934,0.00010061991,0.00005779107,0.0017480243],"genre_scores_gemma":[0.9958417,0.000059764938,0.0038752062,0.000017850742,0.000009466111,0.000005508805,0.00008885896,0.0000040907526,0.00009747211],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999218,0.000013835688,0.000004341411,0.000029248671,0.000014030401,0.000016787611],"domain_scores_gemma":[0.99975246,0.00003450402,0.00007908013,0.000041317806,0.000037274203,0.0000553214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004366477,0.00024697796,0.00020752939,0.0009465024,0.00031183474,0.0009988048,0.00041370696,0.0002793904,0.00042307316],"category_scores_gemma":[0.00038572846,0.00015895162,0.000118198055,0.00041358845,0.00047886383,0.00048365264,0.00044330867,0.0002921481,0.00012299715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014807703,0.00004414711,0.871054,0.000044744458,0.000038466813,0.00015280415,0.0003336226,0.0010930726,0.10494385,0.0011178252,0.00019005762,0.02083937],"study_design_scores_gemma":[0.000005602835,0.000045577515,0.9880713,0.0000082929155,0.000020821442,0.00017631987,0.00017208846,0.00433246,0.0063139377,0.00038457112,0.00046022332,0.000008823066],"about_ca_topic_score_codex":0.0014229836,"about_ca_topic_score_gemma":0.0019283786,"teacher_disagreement_score":0.0014229836,"about_ca_system_score_codex":0.0002898661,"about_ca_system_score_gemma":0.00010698067,"threshold_uncertainty_score":0.0028294325},"labels":[],"label_agreement":null},{"id":"W2817020005","doi":"10.3847/1538-4357/aad332","title":"Detection of Bursts from FRB 121102 with the Effelsberg 100 m Radio Telescope at 5 GHz and the Role of Scintillation","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Scintillation; Fast radio burst; Interstellar medium; Radio telescope; Telescope; Line-of-sight; Galaxy; Optics; Detector","score_opus":0.004368068662125896,"score_gpt":0.2495743715173113,"score_spread":0.2452063028551854,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2817020005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99863213,0.00010138397,0.0004353907,0.000018365803,0.000003660631,0.0000029147154,0.00014678281,0.000024050098,0.00063535565],"genre_scores_gemma":[0.99916756,0.0000333555,0.00034184247,0.000008088044,0.000006160739,0.000002517996,0.00024806987,0.000004900194,0.00018744057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998227,0.00001535156,0.000012998604,0.000055803946,0.000046945093,0.000046274352],"domain_scores_gemma":[0.9994149,0.000111470436,0.00026130272,0.00005839589,0.00006117316,0.000092865725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029364205,0.00024853344,0.00021663224,0.001002531,0.00022421127,0.000489012,0.00031503537,0.00029060687,0.0006446433],"category_scores_gemma":[0.00079454447,0.00017852646,0.00017986861,0.0004721698,0.00020835618,0.00025081873,0.0002953818,0.00025552677,0.00018631689],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028953556,0.000057230343,0.8466475,0.000040544634,0.000075303666,0.0004213565,0.00028802964,0.0007138578,0.14003126,0.00014440368,0.00026239033,0.011028482],"study_design_scores_gemma":[0.0000036602562,0.00004801491,0.9940055,0.0000048306492,0.000015321568,0.0002215637,0.000048212118,0.0007930273,0.004491717,0.00002719139,0.0003351511,0.0000058858022],"about_ca_topic_score_codex":0.0032485116,"about_ca_topic_score_gemma":0.0047796457,"teacher_disagreement_score":0.0032485116,"about_ca_system_score_codex":0.0004038038,"about_ca_system_score_gemma":0.00008675515,"threshold_uncertainty_score":0.006459236},"labels":[],"label_agreement":null},{"id":"W2823209005","doi":"10.3847/1538-4357/aaf230","title":"X-Ray Properties of SPT-selected Galaxy Clusters at 0.2 &lt; z &lt; 1.5 Observed with XMM-Newton","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":126,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astrophysics; Redshift; Halo; Galaxy cluster; Observable; South Pole Telescope; Scaling; Luminosity; Halo mass function; Galaxy; Cluster (spacecraft)","score_opus":0.010429791519988383,"score_gpt":0.1805724123717694,"score_spread":0.17014262085178103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2823209005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992173,0.000011721508,0.000019988382,0.000005690981,5.656473e-7,0.0000016414975,0.0005449396,0.0000056731583,0.00019234825],"genre_scores_gemma":[0.99815553,0.000013411136,0.000044265213,0.000005172495,0.0000027984106,0.000003327597,0.0015733865,0.000003691057,0.00019838804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983406,0.000012866551,0.000011542051,0.000052821568,0.000047204492,0.00004148809],"domain_scores_gemma":[0.9985335,0.00013001215,0.0005542915,0.00012995017,0.000221774,0.00043038715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025144414,0.00023247572,0.00029339717,0.0015408964,0.00040622073,0.00054049667,0.00030042182,0.00021962688,0.0014075219],"category_scores_gemma":[0.0009545653,0.00017386215,0.00022585285,0.0012243825,0.00034021342,0.00031374357,0.00072538236,0.00022572864,0.0005850231],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000630916,0.000010375913,0.9969836,0.0000040922296,0.000019111636,0.00006064578,0.00016119162,0.00017676697,0.0016409575,0.000031157186,0.00017585095,0.00067311176],"study_design_scores_gemma":[7.552375e-7,0.000008501107,0.99971765,3.9965266e-7,0.0000018162912,0.0000209487,0.000036927337,0.00009534923,0.00007021378,0.000003159525,0.00004351909,7.377713e-7],"about_ca_topic_score_codex":0.009502457,"about_ca_topic_score_gemma":0.011348155,"teacher_disagreement_score":0.009502457,"about_ca_system_score_codex":0.0003292001,"about_ca_system_score_gemma":0.00011727016,"threshold_uncertainty_score":0.018894315},"labels":[],"label_agreement":null},{"id":"W283601372","doi":"10.1088/0004-637x/716/1/341","title":"EVOLVING STARBURST MODELING OF FAR-INFRARED/SUBMILLIMETER/MILLIMETER LINE EMISSION. III. APPLICATION TO NEARBY LUMINOUS INFRARED GALAXIES","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Galaxy; Millimeter; Astrophysics; Luminous infrared galaxy; Infrared; Star formation; Far infrared; Submillimeter Array; Astronomy; Luminosity; Line (geometry)","score_opus":0.010100391231737747,"score_gpt":0.2385430178822878,"score_spread":0.22844262665055004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W283601372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8971907,0.00031830225,0.09876629,0.00018297747,0.00002426103,0.000029993824,0.00017957513,0.0001519489,0.003156006],"genre_scores_gemma":[0.9838514,0.0001439144,0.014058412,0.000034180775,0.000014967691,0.000020848865,0.00008045228,0.000037082435,0.0017588255],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995005,0.000011286326,0.0000028507145,0.000017367047,0.000007915185,0.000010599863],"domain_scores_gemma":[0.99982977,0.00004500873,0.000052848554,0.000020915037,0.00002578292,0.000025735431],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025323653,0.00029984865,0.0002862312,0.00017849123,0.00018563205,0.00056444254,0.00081688055,0.0003991256,0.00072994386],"category_scores_gemma":[0.0007046222,0.00021356456,0.00043532567,0.00020152844,0.00024246253,0.00052640605,0.00038543993,0.00033638376,0.00012744902],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003644262,0.00003441826,0.022391563,0.000017060729,0.00003579192,0.0001524422,0.000100734986,0.96367544,0.0042900816,0.003458256,0.00014306954,0.005664598],"study_design_scores_gemma":[0.000002535665,0.000007571448,0.0017113317,0.0000013615011,0.0000049234154,0.000016982001,0.00001332348,0.9971507,0.0002340944,0.00069729437,0.00015783781,0.0000019436964],"about_ca_topic_score_codex":0.013301385,"about_ca_topic_score_gemma":0.007040636,"teacher_disagreement_score":0.013301385,"about_ca_system_score_codex":0.00044194012,"about_ca_system_score_gemma":0.00025674707,"threshold_uncertainty_score":0.026447892},"labels":[],"label_agreement":null},{"id":"W2842352012","doi":"10.3847/1538-4357/aaef8c","title":"Kinematics in Young Star Clusters and Associations with Gaia DR2","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":347,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Astrophysics; Kinematics; Cluster (spacecraft); Star cluster; Star (game theory); Physics; Star formation; Radial velocity; Rotation (mathematics); Astronomy; Stars; Computer science; Geometry; Classical mechanics; Mathematics","score_opus":0.0062086324604896685,"score_gpt":0.21997751841167376,"score_spread":0.2137688859511841,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2842352012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994887,0.00002865339,0.00004380276,0.000004798963,7.9111e-7,0.0000021748792,0.00014151374,0.0000038191624,0.0002856612],"genre_scores_gemma":[0.99878734,0.000020812113,0.00012853579,0.000005033617,0.0000012578536,0.0000026861424,0.00064854155,0.000004058589,0.00040156287],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997844,0.00003574314,0.000012889515,0.00006901541,0.000039283015,0.000058586138],"domain_scores_gemma":[0.9992267,0.00009063351,0.00029913924,0.00008353899,0.00010232932,0.00019776968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038500893,0.00022139336,0.000252932,0.0009991527,0.000362127,0.0006583109,0.0002605012,0.00018298705,0.0011217267],"category_scores_gemma":[0.0009970759,0.00017505352,0.00020509468,0.00066164887,0.00029611686,0.00022981984,0.0008260254,0.00021867178,0.0006261691],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000749485,0.000017902943,0.99633837,0.000003229583,0.000015269114,0.000090957066,0.00017111977,0.000337175,0.001930012,0.00006367904,0.00007746625,0.0008799171],"study_design_scores_gemma":[0.0000030117258,0.000031711857,0.998744,0.0000012052584,0.000005231621,0.00012251799,0.00015735508,0.00037488076,0.00024492654,0.00003483029,0.00027747778,0.0000028195063],"about_ca_topic_score_codex":0.011926615,"about_ca_topic_score_gemma":0.014757491,"teacher_disagreement_score":0.011926615,"about_ca_system_score_codex":0.00037306634,"about_ca_system_score_gemma":0.00019219928,"threshold_uncertainty_score":0.023714423},"labels":[],"label_agreement":null},{"id":"W2844576986","doi":"10.3847/1538-4357/aad2e0","title":"Molecular Gas Filaments and Star-forming Knots Beneath an X-Ray Cavity in RXC J1504–0248","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Canadian Space Agency; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; National Science Council; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Protein filament; Cluster (spacecraft); Star formation; Galaxy; Core (optical fiber); Active galactic nucleus; Molecular cloud; Star cluster","score_opus":0.009861533103677116,"score_gpt":0.25213439950290617,"score_spread":0.24227286639922904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2844576986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994289,0.00008762798,0.000075855234,0.000009901367,0.0000016642718,0.0000030213594,0.00006639293,0.000014743908,0.00031177138],"genre_scores_gemma":[0.9995889,0.000020755984,0.000106121006,0.0000049131704,0.000004972816,0.0000030885342,0.00015573611,0.000002574176,0.000112877664],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999312,0.000006961865,0.0000045894335,0.000018721523,0.000014365176,0.000023983837],"domain_scores_gemma":[0.99975413,0.0000211775,0.00011572755,0.000022891896,0.000029005012,0.000057115485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012596174,0.00017486767,0.00021844108,0.0009064655,0.00027878745,0.00044491867,0.0004458304,0.0003598006,0.0013843101],"category_scores_gemma":[0.00026387532,0.00013069563,0.00018297431,0.00032114005,0.00023366728,0.00024077391,0.0004660495,0.00015811776,0.00029284327],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007646455,0.00016533496,0.7220389,0.00007097683,0.00013804587,0.004315026,0.0007998352,0.0006846706,0.26049072,0.0002908339,0.0005362716,0.009704797],"study_design_scores_gemma":[0.000012393755,0.00007712573,0.996188,0.0000070276333,0.000017048518,0.00050254434,0.00011059674,0.00050767965,0.002032094,0.000037210015,0.00050329475,0.0000050559142],"about_ca_topic_score_codex":0.0029537196,"about_ca_topic_score_gemma":0.002931184,"teacher_disagreement_score":0.0029537196,"about_ca_system_score_codex":0.00025468157,"about_ca_system_score_gemma":0.00005877868,"threshold_uncertainty_score":0.0058730245},"labels":[],"label_agreement":null},{"id":"W2868428220","doi":"10.3847/1538-4357/aad54c","title":"A Dense Companion to the Short-period Millisecond Pulsar Binary PSR J0636+5128","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Millisecond pulsar; Pulsar; Neutron star; Binary pulsar; Orbital period; White dwarf; Pulsar planet; X-ray pulsar; RADIUS","score_opus":0.017245234160639156,"score_gpt":0.3212396398233597,"score_spread":0.3039944056627205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2868428220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988148,0.00004524111,0.00033466393,0.000032445227,0.000005881275,0.0000029578775,0.0000484942,0.000015588234,0.0006999877],"genre_scores_gemma":[0.9996037,0.000009122901,0.00016171932,0.0000065160016,0.0000026644423,7.498524e-7,0.00005474691,0.0000014856355,0.00015930065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999471,0.0000046857785,0.0000035070034,0.000017807857,0.000011861799,0.0000151065315],"domain_scores_gemma":[0.9998135,0.000028770906,0.00006316914,0.000018972423,0.000014145682,0.000061437604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111022026,0.00018709911,0.0001964299,0.00025042397,0.0006301269,0.0005647224,0.00029720293,0.00040110594,0.0016386681],"category_scores_gemma":[0.0004063009,0.00018706237,0.00016711121,0.00022773803,0.00024919971,0.00030145844,0.00049072615,0.00025012164,0.0002745405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074459706,0.0004642853,0.79498947,0.00013140625,0.00013154015,0.005177008,0.0004600174,0.05008177,0.12234365,0.0058421944,0.00215817,0.01747582],"study_design_scores_gemma":[0.000141567,0.0007338486,0.7918352,0.000026874572,0.00007663501,0.004686079,0.00042195152,0.17970055,0.013737844,0.0025559224,0.0060418737,0.00004157841],"about_ca_topic_score_codex":0.0034963326,"about_ca_topic_score_gemma":0.0027699235,"teacher_disagreement_score":0.0034963326,"about_ca_system_score_codex":0.0004647439,"about_ca_system_score_gemma":0.00020215179,"threshold_uncertainty_score":0.006951928},"labels":[],"label_agreement":null},{"id":"W2873976311","doi":"10.3847/1538-4357/aad59a","title":"A Multimessenger Picture of the Flaring Blazar TXS 0506+056: Implications for High-energy Neutrino Emission and Cosmic-Ray Acceleration","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":309,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Blazar; Neutrino; Cosmic ray; Astrophysics; COSMIC cancer database; Astroparticle physics; Neutrino detector; Gamma ray; Nuclear physics; Neutrino oscillation","score_opus":0.009921930287623481,"score_gpt":0.2333763453916099,"score_spread":0.22345441510398642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2873976311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99081475,0.00022905314,0.0018171459,0.00024327158,0.000018052902,0.000009921625,0.0005034469,0.00008496201,0.006279388],"genre_scores_gemma":[0.9980837,0.00005962637,0.0007776274,0.000067006236,0.00001984062,0.0000029218288,0.000554944,0.000014836332,0.0004194291],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990916,0.000007194835,0.0000047639155,0.000035161516,0.000023285778,0.000020441052],"domain_scores_gemma":[0.99978393,0.000030843283,0.00007834867,0.0000417856,0.000024795117,0.000040342788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003069253,0.00038759044,0.00024556305,0.0004073973,0.00052838016,0.0014313523,0.00038217893,0.00042190638,0.0017864566],"category_scores_gemma":[0.00036526847,0.00017550745,0.0004621738,0.00035725167,0.0003981203,0.00047217184,0.0005391851,0.0005712258,0.00021885092],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054379343,0.00016139158,0.85998726,0.00011640862,0.00030116053,0.0012508617,0.00085292285,0.023929643,0.07699592,0.01381006,0.002061294,0.019989245],"study_design_scores_gemma":[0.000030695828,0.00009298901,0.96419805,0.000023404995,0.000054860742,0.0003656499,0.00025123847,0.02392141,0.0044470252,0.003236187,0.003344431,0.000033965847],"about_ca_topic_score_codex":0.0051198946,"about_ca_topic_score_gemma":0.0062650735,"teacher_disagreement_score":0.0051198946,"about_ca_system_score_codex":0.0005497372,"about_ca_system_score_gemma":0.00022261663,"threshold_uncertainty_score":0.010180175},"labels":[],"label_agreement":null},{"id":"W2876555728","doi":"10.3847/1538-4357/aac32a","title":"The Local Cluster Survey. I. Evidence of Outside-in Quenching in Dense Environments","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Halo; Cluster (spacecraft); RADIUS; Galaxy; Galaxy cluster; Quenching (fluorescence); Star formation; Stellar mass; Satellite galaxy","score_opus":0.013200756499168437,"score_gpt":0.24138694347818895,"score_spread":0.22818618697902052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2876555728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974891,0.00010052529,0.000071343835,0.000036913672,0.000001744649,0.000006923047,0.0014430624,0.000020430312,0.000829897],"genre_scores_gemma":[0.99830186,0.00003806576,0.00008040903,0.000024490462,0.000004546775,0.000005512617,0.001220921,0.000007305399,0.00031685957],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973255,0.000033288437,0.000013434068,0.000093610164,0.00004944354,0.000077564044],"domain_scores_gemma":[0.9985557,0.00006683276,0.0005906191,0.00015051891,0.00022047716,0.00041583553],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028722407,0.0001607874,0.00029693442,0.0013858837,0.00077333295,0.00044164681,0.00040654987,0.00020854002,0.001942499],"category_scores_gemma":[0.0006926011,0.0001635832,0.00019865073,0.0013091087,0.0004752265,0.0002636598,0.0008071724,0.00020477637,0.0004408016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007961514,0.000012671625,0.9951023,0.00001942022,0.000029403185,0.000046498622,0.0003309193,0.00008269804,0.0012782605,0.000054042786,0.0007189434,0.0022451228],"study_design_scores_gemma":[0.0000019168676,0.000008077991,0.9995135,0.0000016670052,0.000005989678,0.000019205814,0.00010428143,0.00003785333,0.000075817676,0.000006518266,0.0002232813,0.0000018394612],"about_ca_topic_score_codex":0.062273093,"about_ca_topic_score_gemma":0.104562275,"teacher_disagreement_score":0.062273093,"about_ca_system_score_codex":0.0006498001,"about_ca_system_score_gemma":0.00025961327,"threshold_uncertainty_score":0.12382126},"labels":[],"label_agreement":null},{"id":"W2883201392","doi":"10.3847/1538-4357/aad3c7","title":"Understanding Fundamental Properties and Atmospheric Features of Subdwarfs via a Case Study of SDSS J125637.13–022452.4<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Subdwarf; Luminosity; Stellar classification; Stars; Spectral energy distribution; Bolometer; Spectral line; Line (geometry)","score_opus":0.05405574482439329,"score_gpt":0.24844313271119287,"score_spread":0.19438738788679957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2883201392","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998955,0.000049444774,0.000095506926,0.000020642177,6.602593e-7,0.0000029488506,0.0002566332,0.0000082316765,0.0006108673],"genre_scores_gemma":[0.9988181,0.000032954296,0.00029479153,0.000005395672,0.0000034347647,0.0000012215115,0.0006443459,0.0000058669198,0.00019379013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998908,0.000012328804,0.0000059625704,0.000029203338,0.0000343081,0.00002738543],"domain_scores_gemma":[0.9997104,0.00006812875,0.00007529142,0.000034790326,0.00005100423,0.000060368457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025369786,0.00015641205,0.00015252367,0.001157868,0.0004285815,0.0006364532,0.00025454976,0.00023866181,0.00057792675],"category_scores_gemma":[0.0006063822,0.00006921721,0.00023592493,0.0010551785,0.0003152592,0.00035038716,0.0003881858,0.00018217212,0.00014880314],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018885992,0.0001497517,0.9635597,0.000037052818,0.00005822354,0.0020151525,0.00174084,0.0025317953,0.011637665,0.0009286933,0.00096859597,0.016183784],"study_design_scores_gemma":[0.0000037511033,0.000027949265,0.9911277,0.00000527296,0.000017775192,0.0003008511,0.0011958673,0.003665859,0.0013863984,0.00019527452,0.002065302,0.000007993292],"about_ca_topic_score_codex":0.023054436,"about_ca_topic_score_gemma":0.027113292,"teacher_disagreement_score":0.023054436,"about_ca_system_score_codex":0.0006010987,"about_ca_system_score_gemma":0.000112177826,"threshold_uncertainty_score":0.045840442},"labels":[],"label_agreement":null},{"id":"W2883381102","doi":"10.3847/1538-4357/aaf231","title":"Understanding the Reconstruction of the Biased Tracer","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Quantum Chromodynamics and Particle Interactions","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Perimeter Institute; Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Nonlinear system; Displacement (psychology); Matching (statistics); Noise (video); TRACER; Iterative reconstruction; Mixing (physics); Homogeneous","score_opus":0.033367847041508636,"score_gpt":0.2512478857364834,"score_spread":0.21788003869497474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2883381102","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.21877363,0.00019072229,0.77756256,0.0003541301,0.00003517375,0.00003302217,0.00014608634,0.00033540197,0.0025692324],"genre_scores_gemma":[0.9027307,0.00023260765,0.095005706,0.00006848997,0.00003495011,0.00003509506,0.00019876282,0.00012139379,0.0015722414],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998592,0.000044512188,0.0000059521385,0.000027541235,0.00003341356,0.000029414561],"domain_scores_gemma":[0.99932647,0.00023398157,0.00013773037,0.00009681157,0.0001280527,0.000076982535],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00090705085,0.00030404172,0.00036791948,0.0007258391,0.00031838298,0.0010801506,0.0008323194,0.00087072916,0.0013913626],"category_scores_gemma":[0.0049097952,0.00032772895,0.00023518155,0.00035452252,0.0009907556,0.0018408493,0.0013824411,0.0005307167,0.00030230574],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034794802,0.0000626479,0.018718554,0.00035242172,0.00006666431,0.00082936324,0.0009761441,0.34559682,0.14066277,0.4349434,0.0012398586,0.056203462],"study_design_scores_gemma":[0.000010469183,0.000032558968,0.0021547065,0.0000192799,0.000006891047,0.00013493116,0.00007205317,0.9438698,0.009460957,0.042930774,0.0012867262,0.000020860365],"about_ca_topic_score_codex":0.0016128784,"about_ca_topic_score_gemma":0.00077133,"teacher_disagreement_score":0.0016128784,"about_ca_system_score_codex":0.00058997783,"about_ca_system_score_gemma":0.00062880886,"threshold_uncertainty_score":0.004796982},"labels":[],"label_agreement":null},{"id":"W2883698894","doi":"10.3847/1538-4357/aad4a9","title":"A New Generation of Cool White Dwarf Atmosphere Models. I. Theoretical Framework and Applications to DZ Stars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":99,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Stars; Opacity; Astrophysics; Atmosphere (unit); Spectral line; Helium; Ionization; Effective temperature; Equation of state; Stellar atmosphere; Astronomy; Ion; Atomic physics; Meteorology; Thermodynamics; Quantum mechanics","score_opus":0.013746938405198422,"score_gpt":0.24152532951415726,"score_spread":0.22777839110895884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2883698894","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.23877667,0.0015736758,0.7237795,0.0010786395,0.00032723983,0.00015011925,0.0013538192,0.0019296643,0.03103067],"genre_scores_gemma":[0.81916314,0.0013889509,0.165574,0.0003088165,0.00027766963,0.000301186,0.001262762,0.0010549548,0.010668699],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988735,0.000035407127,0.000006870528,0.000018144361,0.0000392477,0.000012931142],"domain_scores_gemma":[0.99971336,0.00007438496,0.000026176453,0.00006814611,0.000070202026,0.000047628444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003884777,0.0006394437,0.00065072253,0.0004383497,0.0005103148,0.0010122635,0.0013343652,0.00070034695,0.0015582637],"category_scores_gemma":[0.0010994074,0.00033622663,0.0008474959,0.00036477903,0.00049721776,0.00091203,0.0012012172,0.00086030946,0.00046909766],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041465657,0.00005698979,0.0033149268,0.000078742494,0.000066402754,0.00012149395,0.00013131867,0.8973367,0.004835547,0.07904157,0.0016078734,0.013366911],"study_design_scores_gemma":[0.000011898586,0.000010336726,0.00023025145,0.0000060058524,0.0000072453113,0.000015526115,0.0000069588623,0.98767453,0.00029131726,0.008593429,0.0031466587,0.000005893194],"about_ca_topic_score_codex":0.00797952,"about_ca_topic_score_gemma":0.0045523546,"teacher_disagreement_score":0.00797952,"about_ca_system_score_codex":0.0006556039,"about_ca_system_score_gemma":0.00066196744,"threshold_uncertainty_score":0.01586616},"labels":[],"label_agreement":null},{"id":"W2884085396","doi":"10.3847/1538-4357/aae532","title":"A Wildly Flickering Jet in the Black Hole X-Ray Binary MAXI J1535–571","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Labex UnivEarthS; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministerstwo Edukacji i Nauki; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; European Southern Observatory; National Research Foundation; New York University Abu Dhabi; Agence Nationale de la Recherche; National Science Foundation","keywords":"Astrophysics; Physics; Jet (fluid); Black hole (networking); Infrared; Wavelength; Flux (metallurgy); Astronomy; Optics","score_opus":0.016138338525363522,"score_gpt":0.24353656551674704,"score_spread":0.2273982269913835,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2884085396","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99902666,0.00008916653,0.00011935727,0.000012487479,0.0000049733712,0.0000019669587,0.00007177876,0.000010938532,0.00066257763],"genre_scores_gemma":[0.9995521,0.000024824994,0.00010707071,0.000013268767,0.0000069261864,0.0000016716609,0.00013514447,0.0000042718957,0.00015470662],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999449,0.0000034901798,0.0000028304041,0.000017123753,0.000015661037,0.00001597376],"domain_scores_gemma":[0.9998215,0.000018878614,0.000077585675,0.000017066863,0.000018060475,0.000046848167],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011764796,0.00016106102,0.00025623819,0.0004361587,0.00043681986,0.0004665858,0.0001736375,0.00019445292,0.0009465646],"category_scores_gemma":[0.00019293923,0.000107314154,0.00013140692,0.00024560798,0.00023190964,0.00014800673,0.00048111952,0.0002736092,0.00021155248],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001218646,0.00016574081,0.6282563,0.00009238336,0.00011592608,0.0031311226,0.00070344616,0.0005650538,0.34604153,0.00042732139,0.000684438,0.018597977],"study_design_scores_gemma":[0.000006071074,0.00009321195,0.99482673,0.0000057716193,0.000016193855,0.0004362792,0.0001256447,0.00029687205,0.0036934735,0.00004516153,0.00044920022,0.0000053436916],"about_ca_topic_score_codex":0.0013313283,"about_ca_topic_score_gemma":0.0017759292,"teacher_disagreement_score":0.0013313283,"about_ca_system_score_codex":0.00020444159,"about_ca_system_score_gemma":0.000059494367,"threshold_uncertainty_score":0.0031665564},"labels":[],"label_agreement":null},{"id":"W2884094627","doi":"10.3847/1538-4357/aad461","title":"Microphysics of KCl and ZnS Clouds on GJ 1214 b","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Exoplanet; Metallicity; Opacity; Mixing (physics); Spectral line; Condensation; Nucleation; Brown dwarf; Radiative transfer","score_opus":0.009633792211095327,"score_gpt":0.2412420573133192,"score_spread":0.23160826510222388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2884094627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999432,0.000013305667,0.00008547517,0.000026591179,0.0000015823845,0.0000032030805,0.0001129197,0.00003266821,0.0002922675],"genre_scores_gemma":[0.99966204,0.000008717704,0.00008688883,0.000007003303,0.0000011690119,0.0000021765763,0.00015629343,0.000006969728,0.00006865158],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999151,0.000015644926,0.000005767622,0.000021506234,0.000014237315,0.000027820177],"domain_scores_gemma":[0.9998325,0.000042459047,0.000033335327,0.00002035747,0.000021120404,0.00005012693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015756737,0.00049287087,0.00025560084,0.0004444757,0.0004919842,0.00046329794,0.00050270435,0.0006410277,0.00074817054],"category_scores_gemma":[0.0003938903,0.00023236114,0.00051048683,0.00032617417,0.00046464006,0.0003804412,0.0005850652,0.00031839331,0.00010576993],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008431353,0.00026638174,0.40329105,0.00010407752,0.0002267335,0.0015080463,0.0006479732,0.49945712,0.08532079,0.0023194614,0.0013461254,0.004669097],"study_design_scores_gemma":[0.00020849436,0.00021197609,0.3865095,0.000011768977,0.000055022676,0.00009648917,0.0002825964,0.6055544,0.0059929043,0.00043178422,0.00059827254,0.000046787623],"about_ca_topic_score_codex":0.06955725,"about_ca_topic_score_gemma":0.028235126,"teacher_disagreement_score":0.06955725,"about_ca_system_score_codex":0.0013249516,"about_ca_system_score_gemma":0.0003313677,"threshold_uncertainty_score":0.13830477},"labels":[],"label_agreement":null},{"id":"W2884477257","doi":"10.3847/1538-4357/aae7c8","title":"The Dragonfly Nearby Galaxies Survey. V. HST/ACS Observations of 23 Low Surface Brightness Objects in the Fields of NGC 1052, NGC 1084, M96, and NGC 4258","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Surface brightness; Galaxy; Luminosity; Brightness; Surface brightness fluctuation; Dragonfly; Spiral galaxy; Dwarf galaxy","score_opus":0.014348593476999754,"score_gpt":0.2277079912507152,"score_spread":0.21335939777371543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2884477257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964185,0.000095761476,0.000093597875,0.000022397731,0.000002290609,0.000012704309,0.0014722154,0.000056448807,0.0018262096],"genre_scores_gemma":[0.99083626,0.000067104025,0.0008656385,0.000028833076,0.000010755992,0.000017049197,0.006250767,0.000009747571,0.001913855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989057,0.0000075589455,0.0000043333257,0.000038541268,0.000031429896,0.00002760192],"domain_scores_gemma":[0.99974614,0.000018598164,0.00007059885,0.000023656314,0.000024357832,0.00011675781],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014685903,0.00027666733,0.00014008017,0.0020243977,0.00040674696,0.00034098234,0.0002354611,0.000161568,0.0016814619],"category_scores_gemma":[0.0002220337,0.00014165656,0.00011996625,0.0007360524,0.00017619928,0.00027378535,0.00040939826,0.00012276515,0.00035903734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052606553,0.00015253083,0.9016029,0.00005711904,0.000099046054,0.00047641207,0.0008367957,0.0006557454,0.031229274,0.0002330422,0.008360045,0.055770904],"study_design_scores_gemma":[0.00001232709,0.00003514492,0.99593014,0.000005666593,0.000011148244,0.0001398952,0.00011362038,0.00040106438,0.0013388207,0.000013514898,0.001993976,0.000004707314],"about_ca_topic_score_codex":0.024974827,"about_ca_topic_score_gemma":0.07231014,"teacher_disagreement_score":0.024974827,"about_ca_system_score_codex":0.00062313676,"about_ca_system_score_gemma":0.00012351053,"threshold_uncertainty_score":0.049658895},"labels":[],"label_agreement":null},{"id":"W2884591736","doi":"10.3847/1538-4357/aae089","title":"Distances to the Globular Clusters 47 Tucanae and NGC 362 Using Gaia DR2 Parallaxes","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Globular cluster; Parallax; Physics; Stars; Astrophysics; Astronomy; Small Magellanic Cloud; Proper motion; Cosmic distance ladder; Galaxy","score_opus":0.013239758443158854,"score_gpt":0.24371907319349645,"score_spread":0.2304793147503376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2884591736","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98606235,0.00033932936,0.0010332759,0.000071392744,0.000015081024,0.000019157551,0.0037064452,0.00023806935,0.008514979],"genre_scores_gemma":[0.99441,0.0000698412,0.0015485581,0.000018066317,0.0000083828345,0.000009593486,0.003056575,0.000036379668,0.00084261084],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996618,0.000022095019,0.0000109611665,0.000139282,0.00009328815,0.000072557195],"domain_scores_gemma":[0.9993735,0.00006670302,0.00018198647,0.00007692891,0.00015796217,0.00014284322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002647003,0.00040921097,0.0002987256,0.0029321427,0.0008801939,0.0011330082,0.0005597272,0.0004044448,0.0025862628],"category_scores_gemma":[0.0012783835,0.00015308126,0.00027753625,0.002345902,0.00036645224,0.00047715698,0.0010274614,0.00044521733,0.0009549869],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039398286,0.00002896161,0.9333708,0.00009032823,0.000233355,0.00019623757,0.00070898596,0.0145738525,0.015070167,0.002686421,0.004548914,0.028098023],"study_design_scores_gemma":[0.000022297696,0.00003197865,0.98068905,0.000020360896,0.000036606052,0.00009097142,0.00033605832,0.007633222,0.002877032,0.00063809927,0.0075847018,0.000039601193],"about_ca_topic_score_codex":0.21261583,"about_ca_topic_score_gemma":0.19589803,"teacher_disagreement_score":0.21261583,"about_ca_system_score_codex":0.002201903,"about_ca_system_score_gemma":0.00085572654,"threshold_uncertainty_score":0.42275655},"labels":[],"label_agreement":null},{"id":"W2884730008","doi":"10.3847/1538-4357/aad4a2","title":"Multiwavelength Light Curves of Two Remarkable Sagittarius A* Flares","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Supermassive black hole; Astrophysics; Sagittarius A*; Submillimeter Array; Astronomy; Galaxy; Milky Way; Flux (metallurgy); Flare; Galactic Center; Accretion (finance); Black hole (networking); Active galactic nucleus; Star formation","score_opus":0.01262142982167518,"score_gpt":0.25300231196296313,"score_spread":0.24038088214128794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2884730008","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99588543,0.000100997284,0.00034341955,0.00008756029,0.000011611336,0.0000068272548,0.0007985052,0.00008938448,0.0026761298],"genre_scores_gemma":[0.9973833,0.000048639078,0.0003627522,0.00006434843,0.000026575344,0.0000064521696,0.0016312714,0.000018089087,0.00045844738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994516,0.000004535786,0.000003886618,0.000015340036,0.00001483841,0.000016294258],"domain_scores_gemma":[0.9993267,0.00013071753,0.00019981661,0.00004262898,0.000092625625,0.00020748966],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013482077,0.00022755461,0.0001715063,0.0012998272,0.00027021472,0.0002886004,0.00017848391,0.000441771,0.0012054214],"category_scores_gemma":[0.0003908972,0.00010394566,0.00024382053,0.0004978395,0.00012899359,0.00018342918,0.00029181264,0.00047231073,0.00032811752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001063491,0.0003517233,0.76849574,0.00008463664,0.00019592431,0.0018318419,0.0007116202,0.0015594058,0.18691613,0.00070688175,0.004403703,0.033678874],"study_design_scores_gemma":[0.000003199826,0.000053162305,0.99745435,0.0000028672416,0.000007040634,0.0002738319,0.00004936518,0.0007206595,0.00086115213,0.00005844168,0.0005103199,0.000005637199],"about_ca_topic_score_codex":0.002656289,"about_ca_topic_score_gemma":0.003669302,"teacher_disagreement_score":0.002656289,"about_ca_system_score_codex":0.00025466553,"about_ca_system_score_gemma":0.00005080744,"threshold_uncertainty_score":0.005281627},"labels":[],"label_agreement":null},{"id":"W2884767497","doi":"10.3847/1538-4357/aabfe5","title":"Emergence and Variability of Broad Absorption Line Quasar Outflows","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Spectral line; Sky; Observatory; Line (geometry); Flux (metallurgy); Coherence (philosophical gambling strategy); Absorption (acoustics)","score_opus":0.00941862772027493,"score_gpt":0.23297141861303583,"score_spread":0.2235527908927609,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2884767497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99964607,0.000022812428,0.0001027849,0.0000030034353,7.9580303e-7,0.0000016826341,0.00007650748,0.000005830735,0.0001403572],"genre_scores_gemma":[0.9996481,0.0000100532725,0.00007150146,0.0000026571358,0.0000020491282,0.0000011566683,0.00022549917,0.000001506182,0.00003752299],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981695,0.000025825013,0.0000135611745,0.00005972126,0.000031204967,0.000052655392],"domain_scores_gemma":[0.9981566,0.0003455537,0.0008171564,0.00011291302,0.00020003997,0.0003678449],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035134563,0.00014159229,0.00017912802,0.0010605191,0.00025204755,0.00058210024,0.00017643851,0.00016355873,0.00067328324],"category_scores_gemma":[0.0011978004,0.000098359895,0.00017097399,0.00036529457,0.00027626957,0.0002902837,0.00046083337,0.00025236062,0.00012836375],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039322847,0.000027157057,0.9930496,0.0000035472397,0.000015969805,0.00009861459,0.00008564475,0.00007253065,0.0050759343,0.000037199527,0.000034778623,0.0014597013],"study_design_scores_gemma":[7.8527125e-7,0.000016383114,0.99948907,9.60454e-7,0.0000023348975,0.0000719017,0.00005058463,0.00016171433,0.00015879794,0.0000107437845,0.000035518304,0.0000011395301],"about_ca_topic_score_codex":0.0016846925,"about_ca_topic_score_gemma":0.0023628394,"teacher_disagreement_score":0.0016846925,"about_ca_system_score_codex":0.00017501113,"about_ca_system_score_gemma":0.00007647881,"threshold_uncertainty_score":0.0033497214},"labels":[],"label_agreement":null},{"id":"W2885031243","doi":"10.3847/1538-4357/aad054","title":"Offsets of Masers with Respect to the Middle of the Perseus Arm and the Corotation Radius in the Milky Way","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Spiral galaxy; Milky Way; Galactic Center; RADIUS; Astronomy; Angular velocity; Rotation (mathematics); Maser; Galaxy rotation curve; Spiral (railway); Stars; Galaxy; Geometry; Galaxy formation and evolution","score_opus":0.014701846496510086,"score_gpt":0.2199183855082473,"score_spread":0.20521653901173723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885031243","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9795609,0.0014405231,0.0019835122,0.00043474234,0.000092996605,0.00001066822,0.0020104754,0.0011079386,0.013358309],"genre_scores_gemma":[0.9967397,0.000070219525,0.0007447496,0.0000352097,0.00004081967,0.000004670579,0.0009401556,0.00012850465,0.0012959697],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998023,0.000019741756,0.00001126251,0.00009209203,0.000029159039,0.00004552851],"domain_scores_gemma":[0.99869967,0.0002565331,0.0004050809,0.00013317155,0.000298416,0.0002070599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039485292,0.0003408151,0.00030502246,0.0013009092,0.0002532428,0.0008637679,0.0002944977,0.00041068584,0.0038636243],"category_scores_gemma":[0.002281243,0.00023990178,0.00023021811,0.00087540015,0.00026014898,0.0006087822,0.0005853873,0.0004293435,0.0016288434],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002474627,0.00008535953,0.79214513,0.00018719384,0.00021949701,0.0010764467,0.0013604163,0.01062735,0.06686791,0.007982814,0.01115079,0.105822444],"study_design_scores_gemma":[0.00006264148,0.000051831514,0.9790188,0.000030222962,0.00006182524,0.00015275153,0.00020981436,0.0041465033,0.00562479,0.0014303245,0.009174866,0.00003561512],"about_ca_topic_score_codex":0.0060297116,"about_ca_topic_score_gemma":0.006313697,"teacher_disagreement_score":0.0060297116,"about_ca_system_score_codex":0.000835579,"about_ca_system_score_gemma":0.00021930924,"threshold_uncertainty_score":0.012925148},"labels":[],"label_agreement":null},{"id":"W2885169667","doi":"10.3847/1538-4357/aae0f9","title":"Minimum Orbital Period of Precataclysmic Variables","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Subdwarf; White dwarf; Orbital period; Brown dwarf; Primary (astronomy); Common envelope; Stars; Variable star; Orbital elements","score_opus":0.009413556995365276,"score_gpt":0.22388541683658425,"score_spread":0.21447185984121897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885169667","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985726,0.000044163382,0.0005147628,0.000010785034,0.0000019300428,0.0000017816302,0.00017000128,0.00001876285,0.0006652983],"genre_scores_gemma":[0.9993197,0.000012971155,0.00019361213,0.0000016095078,0.0000011860253,0.0000025824022,0.0003218449,0.0000050400186,0.00014151477],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999944,0.000008270616,0.0000028318434,0.000020184234,0.000008025473,0.000016766608],"domain_scores_gemma":[0.9996208,0.00016617286,0.00006912795,0.00004261734,0.00003463731,0.00006662541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023033646,0.00015393946,0.00018354571,0.0004098229,0.0003048547,0.000553982,0.00035815145,0.00016463695,0.002055171],"category_scores_gemma":[0.0012268581,0.00010521566,0.00022746545,0.0002646743,0.00022271962,0.00034058548,0.00031713728,0.00022007295,0.00013109816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009935431,0.00012834206,0.83271784,0.0001348368,0.00013651718,0.00035120032,0.00027002883,0.118095845,0.022623185,0.0061142305,0.0010157987,0.01741859],"study_design_scores_gemma":[0.00013593951,0.0005501709,0.7268081,0.000034943034,0.000120212324,0.00058755843,0.00040886633,0.25066257,0.0102928085,0.0065729576,0.0037883965,0.00003744474],"about_ca_topic_score_codex":0.0030759752,"about_ca_topic_score_gemma":0.0031560818,"teacher_disagreement_score":0.0030759752,"about_ca_system_score_codex":0.000374099,"about_ca_system_score_gemma":0.00021749735,"threshold_uncertainty_score":0.006875217},"labels":[],"label_agreement":null},{"id":"W2885180526","doi":"10.3847/1538-4357/aadb3e","title":"The Planck Cold Clump G108.37-01.06: A Site of Complex Interplay between H ii Regions, Young Clusters, and Filaments","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Star cluster; Protein filament; James Clerk Maxwell Telescope; Star formation; Stars; Molecular cloud; Cluster (spacecraft); H II region; Young stellar object","score_opus":0.016108430523238737,"score_gpt":0.27205259508063256,"score_spread":0.2559441645573938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885180526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987925,0.00005328935,0.00008488095,0.000029668929,0.0000017258456,0.0000041008634,0.00018105516,0.000014246362,0.00083849026],"genre_scores_gemma":[0.9992766,0.000026982147,0.00018774818,0.00002001929,0.0000032730811,0.0000026944333,0.00019841359,0.0000036798695,0.00028064314],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999547,0.000001984795,0.0000011053013,0.000016125416,0.000009718505,0.000016311187],"domain_scores_gemma":[0.9999039,0.000005713687,0.00003639863,0.00000847882,0.000005653026,0.000039965966],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000045498633,0.0001428546,0.00017173374,0.00038450808,0.00048863527,0.00041364916,0.00032534616,0.00018799143,0.0013659409],"category_scores_gemma":[0.00012188242,0.00009284708,0.00006315297,0.00041458715,0.00044202965,0.00020542191,0.00055738556,0.00021896533,0.0003140482],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000335878,0.00004874921,0.83564776,0.00006171324,0.00003883499,0.0023391715,0.0012592135,0.0008495351,0.14327,0.0015357581,0.0017687744,0.01284462],"study_design_scores_gemma":[0.000009502453,0.000026926253,0.9931331,0.000005693749,0.000008049323,0.0004010877,0.00049315253,0.000513416,0.0034246116,0.00029465937,0.0016834086,0.0000063777115],"about_ca_topic_score_codex":0.008609648,"about_ca_topic_score_gemma":0.008735176,"teacher_disagreement_score":0.008609648,"about_ca_system_score_codex":0.00045091525,"about_ca_system_score_gemma":0.00013882332,"threshold_uncertainty_score":0.01711905},"labels":[],"label_agreement":null},{"id":"W2885356567","doi":"10.3847/1538-4357/aaee65","title":"PALFA Single-pulse Pipeline: New Pulsars, Rotating Radio Transients, and a Candidate Fast Radio Burst","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; Max-Planck-Gesellschaft; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; Canadian Centre for Applied Research in Cancer Control; National Science Foundation; Compute Canada; Canarie; McGill University; Canadian Institute for Advanced Research; National Aeronautics and Space Administration","keywords":"Pulsar; Physics; Fast radio burst; Astrophysics; Pulse (music); Population; Sensitivity (control systems); Pipeline (software); Optics; Neutron star; Detector; Computer science","score_opus":0.012718851781137602,"score_gpt":0.2870670993705628,"score_spread":0.2743482475894252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885356567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78819233,0.00018395305,0.15225096,0.00041834768,0.00009861286,0.00043901225,0.0057969964,0.048085034,0.0045346967],"genre_scores_gemma":[0.85698676,0.0000311923,0.13294853,0.00027406393,0.00004310979,0.0003906318,0.0061821486,0.0009304817,0.0022130278],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9994873,0.00009207768,0.000022053568,0.00014986575,0.0001540196,0.00009468405],"domain_scores_gemma":[0.99808747,0.00081318576,0.0001796372,0.00041320635,0.00031512612,0.00019125144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016681929,0.0008088852,0.00049052783,0.00073936896,0.00050128915,0.00059520593,0.0011085396,0.00052272656,0.005201479],"category_scores_gemma":[0.0034045405,0.0006482478,0.0007106514,0.0004560387,0.00032457258,0.00084633584,0.00088422204,0.000783581,0.0012564032],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004120703,0.0011267309,0.30706626,0.00042678812,0.0011927709,0.00095801573,0.0008618381,0.13413237,0.18132228,0.0019457602,0.025882727,0.34096378],"study_design_scores_gemma":[0.0005056805,0.0012508231,0.1994391,0.000021221711,0.00019923075,0.0006068409,0.0001279479,0.6964334,0.084547326,0.0014944146,0.015137076,0.00023695029],"about_ca_topic_score_codex":0.010904338,"about_ca_topic_score_gemma":0.011773709,"teacher_disagreement_score":0.010904338,"about_ca_system_score_codex":0.0007224969,"about_ca_system_score_gemma":0.0009980362,"threshold_uncertainty_score":0.021681726},"labels":[],"label_agreement":null},{"id":"W2885408465","doi":"10.3847/1538-4357/aaf808","title":"HST F160W Imaging of Very Massive Galaxies at 1.5 &lt; z &lt; 3.0: Diversity of Structures and the Effect of Close Pairs on Number Density Estimates","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"National Research Foundation; Danmarks Grundforskningsfond; Space Telescope Science Institute; York University; National Aeronautics and Space Administration","keywords":"Physics; Galaxy; Astrophysics; Radio galaxy; Astronomy; Active galactic nucleus; Diversity (politics)","score_opus":0.003036551056038547,"score_gpt":0.19380892667996955,"score_spread":0.190772375623931,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885408465","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99815947,0.00008459973,0.0006891773,0.000021950667,0.0000021912633,0.000004329447,0.00046505252,0.00004391953,0.00052940653],"genre_scores_gemma":[0.9987942,0.00001899097,0.00047817777,0.000014564202,0.0000047129115,0.000003318532,0.0005572715,0.000012336841,0.00011647767],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963546,0.00004006043,0.000019907622,0.000090325455,0.00013564696,0.000078592275],"domain_scores_gemma":[0.998654,0.00024125594,0.00051136117,0.00016685433,0.00017366129,0.00025288903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007892151,0.00021505724,0.0003611945,0.0019995444,0.0004348543,0.00080803054,0.00050872524,0.00038032082,0.0008703322],"category_scores_gemma":[0.0012324038,0.00023338449,0.00032992839,0.0009895264,0.00037466685,0.00044853427,0.0006837949,0.0003162617,0.0003629693],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001256449,0.000046392728,0.96167696,0.00002415893,0.00007240559,0.00015863779,0.0003224962,0.0010246608,0.028405495,0.00015612651,0.00047644536,0.007510611],"study_design_scores_gemma":[0.0000013127668,0.000007449995,0.9979361,0.000001939522,0.0000067391934,0.000047039906,0.000041581636,0.00077645946,0.0010170626,0.000020005882,0.0001413691,0.0000028845047],"about_ca_topic_score_codex":0.0060148975,"about_ca_topic_score_gemma":0.010178503,"teacher_disagreement_score":0.0060148975,"about_ca_system_score_codex":0.0004316492,"about_ca_system_score_gemma":0.000116243216,"threshold_uncertainty_score":0.011959732},"labels":[],"label_agreement":null},{"id":"W2885437728","doi":"10.3847/1538-4357/aacef9","title":"OGLE-2017-BLG-0537: A Microlensing Event with a Resolvable Lens in ≲5 years from High-resolution Follow-up Observations","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Physics; Event (particle physics); Lens (geology); Resolution (logic); Astrophysics; Astronomy; Optics; Stars","score_opus":0.02253471599994426,"score_gpt":0.22549899964100456,"score_spread":0.2029642836410603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885437728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961713,0.0002894337,0.0007631469,0.000060071332,0.000018810482,0.000018026729,0.0016245005,0.00010911175,0.0009456168],"genre_scores_gemma":[0.9945176,0.000057504483,0.00086007966,0.000042121683,0.000026806056,0.000008600508,0.004136139,0.000024896128,0.00032631276],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962866,0.000017054328,0.000015965254,0.000096838354,0.000111276306,0.00013021223],"domain_scores_gemma":[0.9990451,0.00007776905,0.00030361058,0.00012236073,0.00014327494,0.0003079726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045202728,0.00040989614,0.00072092423,0.0015911759,0.0005665519,0.0011381747,0.0003846683,0.00061050156,0.0009680939],"category_scores_gemma":[0.0006682573,0.00017936886,0.00064182456,0.0012127339,0.00027103288,0.00031813208,0.0009597369,0.000493696,0.0005329936],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073498226,0.00019680372,0.9446865,0.00009175418,0.00034610875,0.006593417,0.00048255333,0.0018052261,0.023114214,0.0004758068,0.0020250573,0.019447554],"study_design_scores_gemma":[0.000020100473,0.000087747634,0.99079084,0.000014180103,0.00009871567,0.0009333087,0.00019786778,0.002824684,0.0020189637,0.00015853367,0.0028295964,0.00002549127],"about_ca_topic_score_codex":0.011231267,"about_ca_topic_score_gemma":0.021225601,"teacher_disagreement_score":0.011231267,"about_ca_system_score_codex":0.0010030852,"about_ca_system_score_gemma":0.0004561367,"threshold_uncertainty_score":0.022331774},"labels":[],"label_agreement":null},{"id":"W2885828152","doi":"10.3847/1538-4357/aad557","title":"A High-resolution Mosaic of the Neutral Hydrogen in the M81 Triplet","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Galaxy; Dark matter; Dark galaxy; Dwarf galaxy; Hydrogen; Baryon; Intergalactic travel; Energetic neutral atom; Telescope","score_opus":0.007854944850736378,"score_gpt":0.20938273790844553,"score_spread":0.20152779305770915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2885828152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99522215,0.00013165374,0.0014046462,0.000016449352,0.0000042765587,0.000009512386,0.0012419252,0.00007244504,0.001896873],"genre_scores_gemma":[0.99360037,0.000054015127,0.0033609183,0.000017027683,0.000010205279,0.0000063302236,0.0024112074,0.000030129933,0.0005098221],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999292,0.0000041439143,0.000002695463,0.0000215018,0.000019981153,0.000022365477],"domain_scores_gemma":[0.9998,0.000015154261,0.000031020772,0.000041424093,0.0000410317,0.00007137578],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009524274,0.00015054515,0.00018730438,0.0007721128,0.00027850372,0.00031084957,0.00010323926,0.00017843457,0.0017962996],"category_scores_gemma":[0.00019572787,0.000121831516,0.0002119852,0.0007831954,0.000098727505,0.00014341266,0.00027311454,0.0001088666,0.00041546524],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005877467,0.0000618497,0.14557207,0.000091246104,0.000114718605,0.0011955458,0.00038672032,0.0026213888,0.8149227,0.0002998274,0.0014804435,0.032665737],"study_design_scores_gemma":[0.000014244285,0.00008366205,0.97199935,0.000010907005,0.00004035063,0.00093758776,0.00024977588,0.003812769,0.018437548,0.00019733213,0.004202307,0.000014178121],"about_ca_topic_score_codex":0.002593238,"about_ca_topic_score_gemma":0.0057916488,"teacher_disagreement_score":0.002593238,"about_ca_system_score_codex":0.00017723827,"about_ca_system_score_gemma":0.00013091865,"threshold_uncertainty_score":0.006009221},"labels":[],"label_agreement":null},{"id":"W2886087594","doi":"10.3847/1538-4357/aadb43","title":"The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS). I. A Pilot Study of the Stellar Populations in NGC 2298 and NGC 3201","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Photometry (optics); Astronomy; Star cluster; Open cluster; Proper motion; Stellar population; Milky Way; Astrometry; Advanced Camera for Surveys; Galaxy; Stars; Star formation","score_opus":0.037559066278156514,"score_gpt":0.2715133975699898,"score_spread":0.2339543312918333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886087594","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99423695,0.000033517703,0.0001420581,0.00002033731,0.000001958419,0.00001785774,0.004404059,0.000023150284,0.0011200155],"genre_scores_gemma":[0.9839438,0.000048480175,0.0017598089,0.00002903903,0.000007519358,0.000028134591,0.012860378,0.000016143122,0.0013068351],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983835,0.000021560232,0.000010719451,0.000051159936,0.000045586505,0.00003266065],"domain_scores_gemma":[0.99968064,0.000017315422,0.00007628442,0.000037644968,0.00007064473,0.00011747949],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028619135,0.00015514885,0.00013948756,0.0011094819,0.0003229475,0.00018546096,0.0002738655,0.00012016947,0.0012311542],"category_scores_gemma":[0.00040099412,0.00008314794,0.00014124277,0.00064385583,0.00013436594,0.00021480232,0.0005698202,0.000104831786,0.00043547506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018095456,0.000039166393,0.9731392,0.000027134527,0.000028232938,0.0001265974,0.00038623728,0.00024652595,0.012643011,0.0001786132,0.0017209982,0.011283423],"study_design_scores_gemma":[0.00000823213,0.000033052638,0.9969229,0.0000030073265,0.0000070423616,0.000049918373,0.00011118624,0.00024636288,0.00061486405,0.000030829902,0.0019706371,0.0000019138038],"about_ca_topic_score_codex":0.020976825,"about_ca_topic_score_gemma":0.0543836,"teacher_disagreement_score":0.020976825,"about_ca_system_score_codex":0.00041715786,"about_ca_system_score_gemma":0.00023857196,"threshold_uncertainty_score":0.041709423},"labels":[],"label_agreement":null},{"id":"W2886256983","doi":"10.3847/1538-4357/aaf1cc","title":"The Massively Accreting Cluster A2029","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; York University; Universities Space Research Association; Princeton University; Alfred P. Sloan Foundation; University of Washington; Goddard Space Flight Center; College of Engineering, Michigan State University; Johns Hopkins University; Ministero dell’Istruzione, dell’Università e della Ricerca; Carnegie Mellon University; Office of Science; Harvard University; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; Brookhaven National Laboratory; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Redshift; Cluster (spacecraft); Galaxy cluster; Galaxy; Scaling; Weak gravitational lensing; Accretion (finance); Galaxy formation and evolution","score_opus":0.005456024842311773,"score_gpt":0.205876320529409,"score_spread":0.2004202956870972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886256983","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998268,0.000030346078,0.00008520107,0.0000206963,0.0000024969943,0.000002318876,0.0001699854,0.000009029626,0.0014120261],"genre_scores_gemma":[0.9987692,0.000019561166,0.00022143342,0.000011624809,0.0000049223104,0.0000018279943,0.00063879497,0.0000022280099,0.00033036337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995387,0.0000051337333,0.000001768095,0.000013057977,0.000011312469,0.000014844909],"domain_scores_gemma":[0.99988616,0.000006216096,0.00002470623,0.0000059236054,0.000014017997,0.000062960826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000063940686,0.00019741998,0.00013910729,0.0004952366,0.0006448332,0.0004070183,0.00021012356,0.00015654156,0.0018029569],"category_scores_gemma":[0.00013879115,0.00007266297,0.00011161955,0.00053473696,0.0001785818,0.00019471806,0.0004703301,0.00013288193,0.0004793027],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072653865,0.00020484523,0.9112347,0.000050980867,0.000087750814,0.0014823565,0.00052169565,0.0025595853,0.05771958,0.002209677,0.0027461152,0.02045608],"study_design_scores_gemma":[0.000016474662,0.000106298794,0.98929477,0.0000088859215,0.0000140381935,0.0004118636,0.00039432172,0.0038967214,0.0015132735,0.0004924391,0.0038412453,0.000009785614],"about_ca_topic_score_codex":0.011336119,"about_ca_topic_score_gemma":0.012455728,"teacher_disagreement_score":0.011336119,"about_ca_system_score_codex":0.00030950466,"about_ca_system_score_gemma":0.0001786109,"threshold_uncertainty_score":0.022540271},"labels":[],"label_agreement":null},{"id":"W2886332711","doi":"10.3847/1538-4357/aad815","title":"A Post-correlation Beamformer for Time-domain Studies of Pulsars and Transients","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; Canadian Institute for Advanced Research","funders":"","keywords":"Pulsar; Beamforming; Phased array; Beam (structure); Radio frequency; Interferometry; Giant Metrewave Radio Telescope","score_opus":0.013851148192075351,"score_gpt":0.3319844876405298,"score_spread":0.31813333944845446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886332711","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.003091179,0.000080785474,0.99590033,0.000043415057,0.000021747137,0.000022147213,0.000058376238,0.00032013952,0.0004618143],"genre_scores_gemma":[0.04377758,0.0002749907,0.9530382,0.000085677646,0.00005144845,0.00014269282,0.00031740195,0.00018426929,0.0021277345],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99957055,0.00014787448,0.00002370839,0.00007219705,0.00014497273,0.000040642575],"domain_scores_gemma":[0.9986712,0.00062025123,0.00012611628,0.00015213586,0.0003816239,0.000048737427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011457447,0.00095123646,0.00045655805,0.00058777933,0.00032441356,0.0007073929,0.0005655033,0.0006972027,0.004586491],"category_scores_gemma":[0.0024851675,0.0004261703,0.00061012345,0.0011163853,0.00041322075,0.00068895106,0.00059633446,0.0007666598,0.0019397453],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038742306,0.00010779152,0.0023428919,0.00023637018,0.00017928191,0.00017366823,0.0001899112,0.22254655,0.17853162,0.018717151,0.00486757,0.5717198],"study_design_scores_gemma":[0.000047826456,0.00017965418,0.004122032,0.000033594675,0.000062175175,0.00019810173,0.000059052163,0.940302,0.037325963,0.005290321,0.012334094,0.000045223263],"about_ca_topic_score_codex":0.0021542185,"about_ca_topic_score_gemma":0.0048603294,"teacher_disagreement_score":0.004586491,"about_ca_system_score_codex":0.00042701102,"about_ca_system_score_gemma":0.0012475769,"threshold_uncertainty_score":0.015343308},"labels":[],"label_agreement":null},{"id":"W2886533588","doi":"10.3847/1538-4357/ab2ae1","title":"PS18kh: A New Tidal Disruption Event with a Non-axisymmetric Accretion Disk","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Max-Planck-Gesellschaft; Queen's University; Chinese Academy of Sciences; Istituto Nazionale di Astrofisica; Durham University; Space Telescope Science Institute; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Center for Cosmology and Astroparticle Physics, Ohio State University; National Central University; Villum Fonden; Science and Technology Facilities Council; Universität Basel; Fermilab; Liverpool John Moores University; University of Minnesota; National Science Foundation; Case Western Reserve University; University of Notre Dame; University of Pittsburgh; Los Alamos National Laboratory; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ohio State University; Drexel University; U.S. Naval Observatory; National Natural Science Foundation of China; U.S. Department of Energy; Smithsonian Institution; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Chinese Academy of Sciences South America Center for Astronomy; Queen's University Belfast; Gordon and Betty Moore Foundation","keywords":"Accretion (finance); Spectral line; Accretion disc; Black-body radiation; RADIUS; Emission spectrum; Line (geometry); Luminosity","score_opus":0.007768584269300716,"score_gpt":0.22953357349960038,"score_spread":0.22176498923029966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886533588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982003,0.000118863856,0.000416733,0.00008342915,0.000015318641,0.000015288402,0.00038107633,0.00005136422,0.00071754836],"genre_scores_gemma":[0.99927217,0.00003614963,0.00018171984,0.000023442704,0.000026601738,0.0000033161677,0.00027180312,0.0000039025813,0.00018097514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999138,0.0000053923263,0.0000080694435,0.000024152378,0.00002031134,0.00002820956],"domain_scores_gemma":[0.9995678,0.000044039,0.00018505832,0.00005536322,0.000024374933,0.00012325532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010030791,0.00029920213,0.00025567517,0.0007386489,0.0005619424,0.00051222934,0.0003806658,0.000491307,0.0013564334],"category_scores_gemma":[0.00039935013,0.00014093173,0.00026539597,0.0005713715,0.00036458537,0.00023183932,0.000604277,0.00033741942,0.00033338426],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084155,0.00020412957,0.8828294,0.00008784419,0.00011440687,0.069747224,0.00062287983,0.001039129,0.024485014,0.0007853057,0.0019091758,0.017333845],"study_design_scores_gemma":[0.000102991435,0.0004841868,0.9195085,0.00002733333,0.00006063887,0.061078034,0.0004315627,0.0031136188,0.0053427005,0.0010419927,0.008781859,0.000026568756],"about_ca_topic_score_codex":0.0020329538,"about_ca_topic_score_gemma":0.0017987484,"teacher_disagreement_score":0.0020329538,"about_ca_system_score_codex":0.00043686837,"about_ca_system_score_gemma":0.00013085599,"threshold_uncertainty_score":0.0045377016},"labels":[],"label_agreement":null},{"id":"W2886534026","doi":"10.3847/1538-4357/aafc27","title":"COLDz: Shape of the CO Luminosity Function at High Redshift and the Cold Gas History of the Universe","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":165,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Science and Technology Facilities Council; National Science Foundation","keywords":"Redshift; Luminosity; Galaxy; Luminosity function; Universe; COSMIC cancer database; Line (geometry); Billion years","score_opus":0.0049561171350462445,"score_gpt":0.16581100824227668,"score_spread":0.16085489110723045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886534026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994558,0.0001821115,0.0018961095,0.000072955176,0.0000038761555,0.0000050212825,0.0010625991,0.00010038716,0.0021190357],"genre_scores_gemma":[0.9989672,0.000020074089,0.0002349018,0.000026024865,0.0000055081214,0.0000018003574,0.000557102,0.000011899913,0.00017558788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997435,0.000029681463,0.0000062401,0.00008552041,0.00007028494,0.00006477311],"domain_scores_gemma":[0.99824226,0.0002674519,0.00066617224,0.0002423357,0.0002303219,0.00035155064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045545134,0.0003015458,0.0003174192,0.0016355187,0.00028532365,0.0007841528,0.0003931807,0.00038176018,0.0014040011],"category_scores_gemma":[0.0011309147,0.00021291558,0.00023886237,0.0007615964,0.0005151736,0.000529566,0.0006064045,0.00040735226,0.00039015952],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014172067,0.000030460917,0.9573659,0.00002373258,0.000070229515,0.00013757107,0.0001464647,0.0010352322,0.032705527,0.0006389228,0.00046817865,0.007236203],"study_design_scores_gemma":[0.0000020349091,0.00001307976,0.996287,0.0000018344117,0.0000056170857,0.000058926293,0.000023828363,0.0010103574,0.0022505466,0.000117898846,0.00022349873,0.0000052931846],"about_ca_topic_score_codex":0.004269874,"about_ca_topic_score_gemma":0.0061525516,"teacher_disagreement_score":0.004269874,"about_ca_system_score_codex":0.00051566394,"about_ca_system_score_gemma":0.00010998391,"threshold_uncertainty_score":0.008490026},"labels":[],"label_agreement":null},{"id":"W2886825213","doi":"10.3847/1538-4357/ab290a","title":"COSMOS-DASH: The Evolution of the Galaxy Size–Mass Relation since z ∼ 3 from New Wide-field WFC3 Imaging Combined with CANDELS/3D-HST","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":207,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Space Telescope Science Institute; National Research Foundation; Danmarks Grundforskningsfond; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Stellar mass; Astronomy; Wide Field Camera 3; Field (mathematics); Cosmos (plant); Star formation; Hubble space telescope","score_opus":0.0035821306447374646,"score_gpt":0.18146889160528792,"score_spread":0.17788676096055045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886825213","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9744183,0.00043188295,0.0012565766,0.0001367528,0.000025289684,0.000011030715,0.01946083,0.00039199117,0.003867272],"genre_scores_gemma":[0.97853935,0.00014343485,0.0013276959,0.00004544597,0.000033106437,0.000012362741,0.019279942,0.00010055252,0.00051800325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997967,0.000019882178,0.00001288456,0.00007771926,0.000058993788,0.000033883225],"domain_scores_gemma":[0.99797434,0.00022334009,0.000703796,0.00022309955,0.00037710663,0.00049822504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00080772943,0.0002447419,0.00025105654,0.0020832561,0.0001748535,0.0008573376,0.00034715133,0.00020613374,0.0019673954],"category_scores_gemma":[0.0019247644,0.00017204549,0.0003000597,0.0017812678,0.00027069973,0.000553128,0.0007098114,0.00036246842,0.0009808895],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014962984,0.000028572062,0.9730752,0.000032148306,0.000075650794,0.0001127928,0.00020688081,0.0009613028,0.0037626622,0.00033812568,0.00541184,0.015845243],"study_design_scores_gemma":[0.000003571242,0.0000071221293,0.99692035,0.000004806062,0.0000073558876,0.000048333906,0.00003386562,0.0006963784,0.00032065483,0.00006357493,0.0018877346,0.0000063452308],"about_ca_topic_score_codex":0.017628014,"about_ca_topic_score_gemma":0.029973982,"teacher_disagreement_score":0.017628014,"about_ca_system_score_codex":0.0004753753,"about_ca_system_score_gemma":0.0002738334,"threshold_uncertainty_score":0.03505081},"labels":[],"label_agreement":null},{"id":"W2886830525","doi":"10.3847/1538-4357/aae5f2","title":"Missing Gamma-Ray Halos and the Need for New Physics in the Gamma-Ray Sky","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Intergalactic travel; Astrophysics; Blazar; Halo; Gamma ray; Cosmic ray; Active galactic nucleus; Radio galaxy; Galaxy; Magnetic field; Galactic halo; Quasar; Redshift","score_opus":0.01935224943781138,"score_gpt":0.25220887669507697,"score_spread":0.23285662725726558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886830525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9895732,0.0010915897,0.0038268776,0.00065771985,0.000037659236,0.000006221509,0.00016043706,0.00011341398,0.0045329314],"genre_scores_gemma":[0.9991271,0.0001142986,0.00041878925,0.00007094728,0.00003071287,0.0000016612958,0.000076662436,0.000011057739,0.00014870729],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998355,0.000028859531,0.000011299076,0.000046040146,0.000039587627,0.000038709873],"domain_scores_gemma":[0.99815756,0.00033068415,0.0006192802,0.00038113852,0.00009515786,0.00041623696],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074155146,0.00027072092,0.00039032655,0.00072943413,0.00044237426,0.0014483961,0.00052365736,0.00036374992,0.003688757],"category_scores_gemma":[0.00197557,0.00018531161,0.00033479367,0.00035592113,0.0015604947,0.0011098689,0.0011372946,0.0005155789,0.00024626713],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013377665,0.00013131717,0.7671902,0.0005518753,0.0005684504,0.003163238,0.0009893986,0.006785257,0.08786507,0.08638012,0.003067002,0.04197038],"study_design_scores_gemma":[0.00009439223,0.00014471741,0.90282476,0.00018777902,0.00021240076,0.002516885,0.0008129138,0.016186748,0.009751366,0.057027236,0.010182323,0.000058492762],"about_ca_topic_score_codex":0.0009108177,"about_ca_topic_score_gemma":0.001026902,"teacher_disagreement_score":0.003688757,"about_ca_system_score_codex":0.00025381858,"about_ca_system_score_gemma":0.00023701416,"threshold_uncertainty_score":0.012340128},"labels":[],"label_agreement":null},{"id":"W2886965433","doi":"10.3847/1538-4357/aad68b","title":"The MAVERIC Survey: A Transitional Millisecond Pulsar Candidate in Terzan 5","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Agence Nationale de la Recherche","keywords":"Millisecond pulsar; Globular cluster; Physics; Astrophysics; Pulsar; Millisecond; Brightness; Astronomy; Luminosity; Cluster (spacecraft); Stars; Galaxy","score_opus":0.01201462158992295,"score_gpt":0.2377650120036674,"score_spread":0.22575039041374445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2886965433","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99875844,0.00011210636,0.00005764641,0.000017032075,0.000002958602,0.0000051150682,0.00013758043,0.000004814813,0.0009043131],"genre_scores_gemma":[0.9988758,0.00008932779,0.0001272052,0.000019113171,0.000005245046,0.0000028329678,0.0005772892,0.0000025897248,0.0003006584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999193,0.000008338744,0.000004119405,0.000024142077,0.000011465773,0.00003255395],"domain_scores_gemma":[0.99974936,0.000014849022,0.00009278569,0.000023425464,0.000026729718,0.00009285421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016872562,0.00017092834,0.00018778615,0.0009944699,0.00037233302,0.0005597838,0.00024108266,0.00014670227,0.00095961714],"category_scores_gemma":[0.0002287615,0.0000765601,0.00011338824,0.00068176957,0.00016252566,0.00017651946,0.000493319,0.00016189893,0.00020603294],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010982883,0.000033994973,0.9810635,0.000017878421,0.000030565363,0.00062467495,0.00040081507,0.000093200564,0.009548429,0.00022301007,0.0003471176,0.007506956],"study_design_scores_gemma":[0.0000034897912,0.00003525923,0.9979208,0.0000051200036,0.000009029206,0.00030923678,0.000270792,0.00007106045,0.00018705944,0.000027999,0.0011586475,0.0000014827158],"about_ca_topic_score_codex":0.005286765,"about_ca_topic_score_gemma":0.013101422,"teacher_disagreement_score":0.005286765,"about_ca_system_score_codex":0.00021175448,"about_ca_system_score_gemma":0.00018793912,"threshold_uncertainty_score":0.010511935},"labels":[],"label_agreement":null},{"id":"W2887291499","doi":"10.3847/1538-4357/aacb79","title":"The CO Luminosity Density at High-z (COLDz) Survey: A Sensitive, Large-area Blind Search for Low-J CO Emission from Cold Gas in the Early Universe with the Karl G. Jansky Very Large Array","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Luminosity function; Luminosity; Star formation; Jansky; Astronomy; Luminous infrared galaxy; Line (geometry); Radio galaxy","score_opus":0.012367922289939019,"score_gpt":0.22912169943288246,"score_spread":0.21675377714294344,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2887291499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98727244,0.0004108048,0.006308761,0.00016274139,0.000013978548,0.00005396542,0.0032690568,0.0003079134,0.002200345],"genre_scores_gemma":[0.9897725,0.00012526054,0.0062483274,0.00010349119,0.000034031535,0.00002752286,0.0027177252,0.00003130101,0.0009399075],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994404,0.00010956058,0.000025664172,0.00016738781,0.00015962617,0.00009736178],"domain_scores_gemma":[0.998852,0.00017621747,0.00030235547,0.00019393,0.00014676794,0.00032868926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00079991855,0.00027940053,0.0003119168,0.0016337765,0.00042129308,0.0007679658,0.0004214379,0.00026667968,0.000861043],"category_scores_gemma":[0.0010269657,0.00023672348,0.00019907641,0.0007883958,0.00031630602,0.00042662676,0.0009244318,0.00023963934,0.00030540716],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019997008,0.000064635184,0.92538595,0.000051142928,0.00012106195,0.0001651421,0.00011145136,0.0010671129,0.042063586,0.00051607576,0.0023382986,0.02791553],"study_design_scores_gemma":[0.000032609078,0.000060536287,0.98592025,0.000009970506,0.000057070145,0.00022127717,0.00011576069,0.0044488213,0.0058559356,0.0002919884,0.0029653916,0.00002024145],"about_ca_topic_score_codex":0.006117041,"about_ca_topic_score_gemma":0.017549535,"teacher_disagreement_score":0.006117041,"about_ca_system_score_codex":0.00037204917,"about_ca_system_score_gemma":0.00036731455,"threshold_uncertainty_score":0.012162864},"labels":[],"label_agreement":null},{"id":"W2887658899","doi":"10.3847/1538-4357/aad6dd","title":"A Galaxy-scale Fountain of Cold Molecular Gas Pumped by a Black Hole","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; University of Waterloo","funders":"Office of Naval Research; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; Smithsonian Institution; National Science Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Fountain; Astrophysics; Galaxy; Astronomy; Scale (ratio); Quantum mechanics","score_opus":0.004405336168046818,"score_gpt":0.23382177699549928,"score_spread":0.22941644082745247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2887658899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99863774,0.00005062818,0.00021299736,0.000063905485,0.0000070500496,0.0000025241623,0.000109545275,0.00005376621,0.00086193706],"genre_scores_gemma":[0.9995604,0.000010468005,0.00017503288,0.000021431562,0.000005537218,8.353876e-7,0.00007491374,0.0000037851332,0.00014759277],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999616,0.0000027033868,9.25963e-7,0.000011060032,0.000008795662,0.000014839078],"domain_scores_gemma":[0.9998104,0.00001643021,0.000055652436,0.000032777556,0.000013879248,0.000070919814],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007330941,0.00012124637,0.000169852,0.00041297288,0.0005359649,0.0003193695,0.0002459365,0.00022075765,0.00088682974],"category_scores_gemma":[0.00018154667,0.00008700975,0.00015256701,0.00017399782,0.00035820898,0.00024983636,0.00044981771,0.00025581027,0.00012554805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011579272,0.00019881479,0.71957296,0.0000820244,0.0002996865,0.0058260392,0.0032075765,0.0015564779,0.23597926,0.0027670187,0.005076883,0.024275357],"study_design_scores_gemma":[0.000011444535,0.00009621805,0.9879588,0.000008174759,0.000023146504,0.0005154692,0.00040427336,0.0025389178,0.0057471716,0.00030361203,0.002382167,0.000010499172],"about_ca_topic_score_codex":0.0063142506,"about_ca_topic_score_gemma":0.007241722,"teacher_disagreement_score":0.0063142506,"about_ca_system_score_codex":0.0003823854,"about_ca_system_score_gemma":0.000073674055,"threshold_uncertainty_score":0.012555003},"labels":[],"label_agreement":null},{"id":"W2887865904","doi":"10.3847/1538-4357/aade48","title":"Evolutionary Models for 15 Galactic Supernova Remnants with New Distances","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Supernova; Galaxy; Large Magellanic Cloud; Line (geometry); Milky Way; Interstellar medium; Near-Earth supernova; Supernova remnant; Molecular cloud","score_opus":0.01528409187065779,"score_gpt":0.23446927258083347,"score_spread":0.21918518071017568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2887865904","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9164892,0.00043964293,0.07127183,0.00034746592,0.000040375948,0.000080721125,0.00043312836,0.0002419855,0.010655678],"genre_scores_gemma":[0.9875501,0.00028634627,0.004527531,0.000044907018,0.000023298988,0.0000660421,0.00050379283,0.00007713317,0.006920856],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99974567,0.000062186475,0.000020645793,0.000070836606,0.0000412145,0.000059475282],"domain_scores_gemma":[0.99898154,0.00023838879,0.00032193185,0.00009039774,0.00013857926,0.00022913801],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013779773,0.000630545,0.00056671526,0.001154853,0.0006164646,0.0017847634,0.0022536714,0.00091404794,0.0037369945],"category_scores_gemma":[0.0027702926,0.0006424378,0.0018166354,0.0005475445,0.0010778275,0.0010554016,0.0013467445,0.0006746289,0.0010711051],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013915652,0.000059345934,0.062121894,0.00004622496,0.00018500727,0.0011977301,0.00040001547,0.84368753,0.0018405126,0.08338997,0.000643214,0.0062893922],"study_design_scores_gemma":[0.000055468074,0.000037294092,0.008256695,0.000016964595,0.00006765852,0.00036633344,0.00011186335,0.97397625,0.00027545646,0.015510758,0.0012947592,0.000030452431],"about_ca_topic_score_codex":0.016627792,"about_ca_topic_score_gemma":0.008175064,"teacher_disagreement_score":0.016627792,"about_ca_system_score_codex":0.0017965484,"about_ca_system_score_gemma":0.00071058504,"threshold_uncertainty_score":0.03306198},"labels":[],"label_agreement":null},{"id":"W2887909489","doi":"10.3847/1538-4357/aadee6","title":"The z = 0.54 LoBAL Quasar SDSS J085053.12+445122.5. I. Spectral Synthesis Analysis Reveals a Massive Outflow<sup>∗</sup>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Quasar; Outflow; Redshift; Spectral line; Torus; Metallicity; Photoionization; Halo; Ionization; Astronomy; Stars; Galaxy; Geometry","score_opus":0.007717740760052951,"score_gpt":0.22088495579692757,"score_spread":0.21316721503687464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2887909489","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913406,0.000054840813,0.0033033227,0.000046703706,0.000008562428,0.000013428596,0.002784494,0.00044945304,0.0019987687],"genre_scores_gemma":[0.9928439,0.00001252417,0.0032721083,0.000019650348,0.0000067787046,0.000005914397,0.0034209788,0.000036809986,0.00038128506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999603,0.000004005948,0.000002280719,0.000011153515,0.000013097422,0.000009144399],"domain_scores_gemma":[0.99989164,0.000019395427,0.000028774746,0.000012810454,0.000023480783,0.000023982133],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016876488,0.00019514908,0.00010328929,0.00079695624,0.00021814699,0.00031933904,0.00016923026,0.00013189702,0.0021666493],"category_scores_gemma":[0.00020512557,0.0000776762,0.00024422418,0.0003295191,0.00011578611,0.00009624805,0.0001681747,0.000112267284,0.0005002507],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007892686,0.0001964197,0.65914524,0.0001500965,0.00017190211,0.001075091,0.00038357626,0.018707668,0.25579298,0.003224055,0.0055379537,0.054825712],"study_design_scores_gemma":[0.00003616077,0.00007278746,0.9351589,0.0000063300718,0.000039399354,0.00019763487,0.00023741007,0.04264954,0.016879532,0.0008623392,0.0038435739,0.000016416421],"about_ca_topic_score_codex":0.0037458064,"about_ca_topic_score_gemma":0.0046369643,"teacher_disagreement_score":0.0037458064,"about_ca_system_score_codex":0.00023824691,"about_ca_system_score_gemma":0.000071322094,"threshold_uncertainty_score":0.007447958},"labels":[],"label_agreement":null},{"id":"W2888035497","doi":"10.3847/1538-4357/aaf4bc","title":"Joint Power Spectrum and Voxel Intensity Distribution Forecast on the CO Luminosity Function with COMAP","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Markov chain Monte Carlo; Luminosity; Monte Carlo method; Halo; Covariance; Luminosity function; Spectral density; Statistical physics; Astrophysics; Statistics; Galaxy; Mathematics","score_opus":0.007059563967924559,"score_gpt":0.18014016927652013,"score_spread":0.17308060530859556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2888035497","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.37713692,0.00014884438,0.6141589,0.00062566396,0.0000361344,0.00006747293,0.0008755189,0.0014102164,0.0055402955],"genre_scores_gemma":[0.9611037,0.000030559113,0.03739308,0.000068063324,0.00002408625,0.000048196514,0.0004924316,0.0001855746,0.0006542924],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99940896,0.0002215366,0.000022090631,0.00013086862,0.00013466571,0.00008196378],"domain_scores_gemma":[0.99529475,0.0027533679,0.0005124312,0.00053378055,0.0005715204,0.0003340705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027505436,0.0005160253,0.00084721093,0.0008401405,0.00061351864,0.0012124509,0.0014517073,0.00075337006,0.0029689048],"category_scores_gemma":[0.014321043,0.00081153837,0.0007138528,0.00066568743,0.0011275101,0.001765256,0.0014152088,0.0011370449,0.00033337885],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006949201,0.000016770973,0.00837215,0.000010843873,0.000027947557,0.000041431038,0.000034958342,0.97241926,0.0006295203,0.012675621,0.00052049494,0.005181472],"study_design_scores_gemma":[0.000010116202,0.0000059968193,0.0010606124,0.000002500218,0.0000027821866,0.000007103302,0.0000052567875,0.993757,0.0002337616,0.004752866,0.00015427804,0.000007701406],"about_ca_topic_score_codex":0.025532953,"about_ca_topic_score_gemma":0.017480731,"teacher_disagreement_score":0.025532953,"about_ca_system_score_codex":0.0014343495,"about_ca_system_score_gemma":0.001835901,"threshold_uncertainty_score":0.050768673},"labels":[],"label_agreement":null},{"id":"W2888069498","doi":"10.3847/1538-4357/aadadd","title":"Multiple Disk Gaps and Rings Generated by a Single Super-Earth. II. Spacings, Depths, and Number of Gaps, with Application to Real Systems","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Planet; Millimeter; Instability; Planetary mass; Mars Exploration Program; Metric (unit); Planetary system; Terrestrial planet","score_opus":0.00596641497157204,"score_gpt":0.21744646336214912,"score_spread":0.21148004839057707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2888069498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956974,0.0002027108,0.0033044466,0.0000583121,0.0000051180214,0.000011589409,0.00018593577,0.00008710031,0.00044738353],"genre_scores_gemma":[0.9976927,0.00003177142,0.0021399283,0.0000036243136,0.0000045606635,0.00000306972,0.000073684176,0.00000859915,0.000042087762],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996731,0.000100887875,0.000020489033,0.000120633034,0.000048852253,0.0000359711],"domain_scores_gemma":[0.9915605,0.0054326886,0.0015421995,0.00069449795,0.0004583748,0.00031168546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010626839,0.00039721045,0.0002971542,0.0010265738,0.0005838391,0.0009901079,0.00073606503,0.0009825334,0.0008023408],"category_scores_gemma":[0.008501418,0.00034965805,0.00035985187,0.0007527285,0.0009098003,0.0013007444,0.0006244688,0.0004801347,0.00013418886],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058648613,0.00025659695,0.38571683,0.00036497405,0.00012119117,0.0013331088,0.00054216123,0.5574526,0.020851897,0.004487043,0.0007978056,0.02748922],"study_design_scores_gemma":[0.000027340911,0.000113048474,0.09347228,0.000020953448,0.000022919034,0.00056979764,0.00026076005,0.8969889,0.005743548,0.0023031337,0.0004387303,0.000038626935],"about_ca_topic_score_codex":0.0031161874,"about_ca_topic_score_gemma":0.002071903,"teacher_disagreement_score":0.0031161874,"about_ca_system_score_codex":0.0008867461,"about_ca_system_score_gemma":0.00018295442,"threshold_uncertainty_score":0.006433904},"labels":[],"label_agreement":null},{"id":"W2888214738","doi":"10.3847/1538-4357/ab01fd","title":"The NANOGrav 11 yr Data Set: Solar Wind Sounding through Pulsar Timing","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"","keywords":"Pulsar; Millisecond pulsar; Observatory; Solar wind; Sky; Variation (astronomy); Interstellar medium; Gravitational wave","score_opus":0.04285195722990756,"score_gpt":0.3557894128572232,"score_spread":0.3129374556273157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2888214738","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5266939,0.0007138645,0.0030194814,0.00041178064,0.00022484572,0.00011891547,0.45547226,0.00091653096,0.0124284215],"genre_scores_gemma":[0.3484836,0.00022094024,0.003951001,0.00013905467,0.00011739711,0.00015444368,0.64317036,0.00016898416,0.003594209],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994497,0.000065674576,0.00008419885,0.00013401013,0.00021882071,0.00004759345],"domain_scores_gemma":[0.99826485,0.00028132397,0.00035079184,0.0006219244,0.00033492362,0.00014628269],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006828959,0.0003596996,0.00041059148,0.0018301524,0.00035786405,0.0007554348,0.000570751,0.0003835089,0.0033981185],"category_scores_gemma":[0.0017616273,0.00016356604,0.00028507647,0.0026812674,0.00023709146,0.0004297333,0.0009015356,0.0003824481,0.0027818352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016419077,0.00041387553,0.72297233,0.0005822412,0.0005979332,0.0008557347,0.00044072492,0.010266642,0.02070106,0.0026264272,0.16193374,0.07696745],"study_design_scores_gemma":[0.00019548423,0.00021004582,0.8401454,0.00007290167,0.000083623156,0.00039356432,0.00024644894,0.007443349,0.004795866,0.00076772243,0.14559413,0.000051525807],"about_ca_topic_score_codex":0.0065855244,"about_ca_topic_score_gemma":0.013484384,"teacher_disagreement_score":0.0065855244,"about_ca_system_score_codex":0.00021989635,"about_ca_system_score_gemma":0.00031218128,"threshold_uncertainty_score":0.013094425},"labels":[],"label_agreement":null},{"id":"W2888520146","doi":"10.3847/1538-4357/aadc0c","title":"Confirmation Of Two Galactic Supernova Remnant Candidates Discovered by THOR","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Supernova; Supernova remnant; Physics; Pulsar; Milky Way; Astrophysics; Spectral index; Polarization (electrochemistry); Synchrotron; Astronomy; Galaxy; Spectral line; Optics","score_opus":0.007960531927622798,"score_gpt":0.2451739887669667,"score_spread":0.2372134568393439,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2888520146","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99348193,0.0008455748,0.0010445717,0.00035386527,0.0002589573,0.000030208248,0.00024074162,0.00006766143,0.0036764264],"genre_scores_gemma":[0.99805474,0.00017604625,0.00071728294,0.00013505467,0.00005640412,0.0000038436015,0.00019527249,0.000009024392,0.00065237307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995541,0.00005563695,0.00008071862,0.00010594712,0.00007755737,0.00012604085],"domain_scores_gemma":[0.997666,0.0004875647,0.00040926223,0.00039913712,0.0005135036,0.00052450126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014996314,0.0005178519,0.00037590793,0.0019327116,0.0010423283,0.0011993004,0.00081670034,0.0011522899,0.0027097848],"category_scores_gemma":[0.0044047106,0.00034798135,0.000777426,0.00048380202,0.0008741324,0.00047655424,0.0010718885,0.00067338883,0.001057831],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011474033,0.00022750143,0.83313334,0.00014296582,0.00017723929,0.121847376,0.0009394808,0.00022585825,0.025930956,0.0024911514,0.0014647219,0.012272051],"study_design_scores_gemma":[0.0002174234,0.0012756521,0.6391445,0.00015261902,0.00033222325,0.2858727,0.0024165644,0.003159809,0.044441573,0.0013283647,0.02157953,0.00007906007],"about_ca_topic_score_codex":0.0027442873,"about_ca_topic_score_gemma":0.0018734569,"teacher_disagreement_score":0.0027442873,"about_ca_system_score_codex":0.00035074976,"about_ca_system_score_gemma":0.00037822087,"threshold_uncertainty_score":0.009065092},"labels":[],"label_agreement":null},{"id":"W2888591728","doi":"10.3847/1538-4357/aadd18","title":"SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). II. Structural Properties and Near-infrared Morphologies of Faint Submillimeter Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Japan Society for the Promotion of Science; Ministry of Science and Technology, Taiwan; Chinese Academy of Sciences; National Natural Science Foundation of China; National Key Research and Development Program of China; Science and Technology Facilities Council; National Astronomical Observatory of Japan; European Commission; Academia Sinica; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Narodowym Centrum Nauki; National Science Foundation","keywords":"Galaxy; Stellar mass; Star formation; Redshift; Luminosity; Luminous infrared galaxy; Spectral energy distribution","score_opus":0.021869847353448577,"score_gpt":0.23512590694873622,"score_spread":0.21325605959528765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2888591728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.977097,0.0002458971,0.00021497863,0.000044505512,0.0000060290113,0.00003769451,0.017411634,0.00007721942,0.0048650177],"genre_scores_gemma":[0.9464254,0.00016576998,0.0012053923,0.00005725859,0.000025100884,0.00004287963,0.04961558,0.000036868547,0.002425787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998816,0.000014940553,0.000008778459,0.000030127374,0.000030403537,0.000034035995],"domain_scores_gemma":[0.9994512,0.00003122349,0.00015894616,0.00006522596,0.0001165045,0.00017685602],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020710558,0.00024589105,0.00014715493,0.0027179732,0.00025342542,0.0003985564,0.0002510836,0.00013189563,0.0019075975],"category_scores_gemma":[0.00038583035,0.000103560895,0.00020268312,0.0017874466,0.00011117723,0.00024143458,0.00042975217,0.00014219912,0.00063510495],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015099453,0.000034124776,0.9800837,0.000032155367,0.000049387087,0.00008681386,0.00010077924,0.00014396227,0.006047127,0.00015319181,0.0030004287,0.010117214],"study_design_scores_gemma":[0.000005008266,0.0000074631344,0.99794346,0.0000036098036,0.000007857602,0.000045916047,0.00004045428,0.00015735421,0.00029224245,0.000014328554,0.0014808743,0.0000013582644],"about_ca_topic_score_codex":0.019288426,"about_ca_topic_score_gemma":0.044281807,"teacher_disagreement_score":0.019288426,"about_ca_system_score_codex":0.00025378252,"about_ca_system_score_gemma":0.00026405853,"threshold_uncertainty_score":0.03835231},"labels":[],"label_agreement":null},{"id":"W2889032074","doi":"10.3847/1538-4357/aadd95","title":"Authenticating the Presence of a Relativistic Massive Black Hole Binary in OJ 287 Using Its General Relativity Centenary Flare: Improved Orbital Parameters","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Positive Living North","funders":"Science and Technology Facilities Council","keywords":"Physics; Gravitational wave; Astrophysics; Blazar; Flare; Black hole (networking); Relativistic quantum chemistry; Binary black hole; Theory of relativity; Quadrupole; General relativity; Astronomy; Binary number; Theoretical physics; Quantum mechanics; Gamma ray","score_opus":0.024210026125452703,"score_gpt":0.3178134677366292,"score_spread":0.2936034416111765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889032074","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99825424,0.000030199375,0.0006247674,0.000014559715,0.0000034090228,0.000005541972,0.000073868934,0.000015939986,0.0009773369],"genre_scores_gemma":[0.99960035,0.000008725483,0.00027595685,0.000003150784,0.0000016097971,5.918866e-7,0.000051535444,0.0000020234556,0.00005602454],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999589,0.0000037161296,0.0000024389017,0.000010398366,0.000013368685,0.000011333712],"domain_scores_gemma":[0.99975735,0.000026856414,0.000115984585,0.000036283538,0.0000205152,0.00004310651],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028342954,0.00015004657,0.00016244726,0.00046641615,0.00029185216,0.00055927364,0.00021990913,0.00013757,0.0008187024],"category_scores_gemma":[0.00050939195,0.0000812384,0.00011544215,0.0003522965,0.00030444836,0.00017881216,0.00049226655,0.00024634134,0.00013260067],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003810754,0.000070334725,0.8988644,0.00007267696,0.0000736992,0.0008837454,0.00041668152,0.0031285768,0.0748231,0.0022579595,0.00029836307,0.018729411],"study_design_scores_gemma":[0.000023565537,0.00015497983,0.9763716,0.000009800615,0.000065985754,0.0004592904,0.00032022045,0.0108796945,0.010066172,0.00058945233,0.0010394887,0.000019765675],"about_ca_topic_score_codex":0.0049752397,"about_ca_topic_score_gemma":0.008387292,"teacher_disagreement_score":0.0049752397,"about_ca_system_score_codex":0.00029569987,"about_ca_system_score_gemma":0.00019054137,"threshold_uncertainty_score":0.009892523},"labels":[],"label_agreement":null},{"id":"W2889248467","doi":"10.3847/1538-4357/aadcff","title":"The Scattering and Intrinsic Structure of Sagittarius A* at Radio Wavelengths","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":101,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council; Russian Academy of Sciences; Harvard University; Swinburne University of Technology; Gordon and Betty Moore Foundation; John Templeton Foundation; National Science Foundation","keywords":"Physics; Sagittarius A*; Scattering; Astrophysics; Galactic Center; Angular diameter; Supermassive black hole; Computational physics; Galaxy; Quantum mechanics; Stars","score_opus":0.007116505746994845,"score_gpt":0.21481477708582275,"score_spread":0.2076982713388279,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889248467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99916077,0.000018955845,0.00021831605,0.000007345063,7.5950743e-7,7.148016e-7,0.00007641799,0.000018687395,0.00049807393],"genre_scores_gemma":[0.9996106,0.000009868849,0.00009112143,0.000003770814,0.0000020479476,7.448961e-7,0.0002342312,0.000006433871,0.00004123574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.000009206145,0.0000046739488,0.000017643115,0.000014810451,0.000016766187],"domain_scores_gemma":[0.9995442,0.000056698027,0.00017703515,0.00004156345,0.0000844936,0.00009591093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015097915,0.0002692968,0.00013083777,0.00071844354,0.00024604934,0.00047945214,0.00024033607,0.00017063995,0.0004711301],"category_scores_gemma":[0.00040452427,0.00015270965,0.00021145771,0.00032156956,0.00025784288,0.00023857605,0.00027627297,0.00013171502,0.00020080304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015301318,0.00004792235,0.8879861,0.00002488755,0.00013314708,0.00026554338,0.00028057297,0.005087447,0.09759645,0.0010423184,0.00037393966,0.007008528],"study_design_scores_gemma":[0.0000029909418,0.000025541842,0.9914621,0.0000023478633,0.000012013331,0.000070589296,0.00006535632,0.0065015214,0.0015457643,0.00015372473,0.0001524361,0.0000056112685],"about_ca_topic_score_codex":0.0038548987,"about_ca_topic_score_gemma":0.00300917,"teacher_disagreement_score":0.0038548987,"about_ca_system_score_codex":0.00032020514,"about_ca_system_score_gemma":0.00006774628,"threshold_uncertainty_score":0.007664919},"labels":[],"label_agreement":null},{"id":"W2889433878","doi":"10.3847/1538-4357/aadcfe","title":"Infrared Variability of Two Dusty White Dwarfs","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"White dwarf; Planetesimal; Infrared; Circumstellar dust; Infrared excess; Flux (metallurgy); Cosmic dust; Perturbation (astronomy)","score_opus":0.010202037162044144,"score_gpt":0.2546181662805049,"score_spread":0.24441612911846072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889433878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99966574,0.000014102121,0.000028200948,0.0000036686854,0.0000012535397,0.0000012288393,0.00007119815,0.000003756259,0.00021080131],"genre_scores_gemma":[0.9995696,0.0000056311073,0.00004532978,0.000004130428,0.0000020513567,0.0000012654492,0.00024214636,0.0000010262121,0.00012879331],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998925,0.0000066863445,0.0000075399385,0.000044733988,0.00002313805,0.00002542243],"domain_scores_gemma":[0.999716,0.000019925768,0.00008807009,0.00001678294,0.000051500723,0.00010776022],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013795437,0.00017394855,0.0001720445,0.0006979313,0.00031115912,0.00031754482,0.00018363551,0.00022844352,0.00047665535],"category_scores_gemma":[0.00027125495,0.000061890525,0.00010643882,0.00036354657,0.00020659063,0.00014979069,0.0002736653,0.00013189601,0.00017033385],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015566472,0.00007452865,0.9528817,0.000008970888,0.000023722241,0.0003209657,0.00033876658,0.00009698867,0.043091446,0.00007847172,0.00015934539,0.0027694295],"study_design_scores_gemma":[0.0000020126631,0.000027453616,0.9983011,6.8349016e-7,0.0000044632875,0.00012879854,0.00009214003,0.00011093412,0.0010672082,0.000012290059,0.00025152724,0.0000013913683],"about_ca_topic_score_codex":0.0041729105,"about_ca_topic_score_gemma":0.0049002133,"teacher_disagreement_score":0.0041729105,"about_ca_system_score_codex":0.00032568257,"about_ca_system_score_gemma":0.00007603132,"threshold_uncertainty_score":0.008297265},"labels":[],"label_agreement":null},{"id":"W2889460758","doi":"10.3847/1538-4357/aade4e","title":"VERITAS and Fermi-LAT Observations of TeV Gamma-Ray Sources Discovered by HAWC in the 2HWC Catalog","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cherenkov radiation; Pulsar; Astroparticle physics; Pulsar wind nebula; Crab Nebula; Source counts; High energy","score_opus":0.012998755711662155,"score_gpt":0.22450142989594873,"score_spread":0.2115026741842866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889460758","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97926563,0.0008048763,0.0007670361,0.00008805219,0.000027470163,0.00004447818,0.011972112,0.0002984733,0.0067318697],"genre_scores_gemma":[0.9455286,0.00040830803,0.002315374,0.00020299507,0.00008813109,0.00006777433,0.0490156,0.00011985815,0.0022532907],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959785,0.000023508586,0.000029255152,0.000101028934,0.00013705097,0.000111332636],"domain_scores_gemma":[0.9974245,0.00031351438,0.0008312436,0.0005941967,0.00046729724,0.0003692873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007291513,0.0002647543,0.00029819747,0.005928585,0.0005322506,0.00084100803,0.00043232826,0.00026795783,0.0034358306],"category_scores_gemma":[0.0014074798,0.00018128254,0.00025361587,0.0027823588,0.000218307,0.00045462154,0.0011255115,0.0002424759,0.0008941823],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002905094,0.000053864693,0.933903,0.00008675312,0.00011514818,0.00081206573,0.0004457377,0.0002519576,0.009858676,0.0006497561,0.009465624,0.044067],"study_design_scores_gemma":[0.000020841635,0.000030277874,0.9854235,0.000034869965,0.000030351479,0.00055285887,0.00012246762,0.00039650837,0.0021232734,0.00013414171,0.0111177275,0.000013025357],"about_ca_topic_score_codex":0.008029028,"about_ca_topic_score_gemma":0.0153318085,"teacher_disagreement_score":0.008029028,"about_ca_system_score_codex":0.0005678347,"about_ca_system_score_gemma":0.00039751027,"threshold_uncertainty_score":0.015964568},"labels":[],"label_agreement":null},{"id":"W2889547825","doi":"10.3847/1538-4357/aad4b3","title":"The Unexpected Kinematics of Multiple Populations in NGC 6362: Do Binaries Play a Role?*","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Leverhulme Trust","keywords":"Physics; Astrophysics; Globular cluster; Stars; Velocity dispersion; Dispersion (optics); Kinematics; Population; Radial velocity; Binary number; Stellar kinematics; Cluster (spacecraft); Anisotropy; Galaxy; Milky Way; Classical mechanics; Optics","score_opus":0.01748219554185323,"score_gpt":0.2536833815688346,"score_spread":0.23620118602698134,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2889547825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99816567,0.00012993401,0.0010992986,0.00003678691,0.0000040086175,0.0000016769038,0.00005659721,0.000026907976,0.00047918592],"genre_scores_gemma":[0.9994717,0.000022848291,0.00033653923,0.000006648395,0.0000031470722,0.0000012214451,0.000050969546,0.0000074506506,0.000099553225],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993634,0.000008536115,0.0000033537756,0.000022880657,0.00001274668,0.000016170086],"domain_scores_gemma":[0.9998318,0.000037213154,0.00004439299,0.000024829125,0.00001560915,0.000046229252],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026034375,0.00020535357,0.00036161178,0.00035110657,0.0003806371,0.0007609853,0.0003004734,0.00030769172,0.0012372567],"category_scores_gemma":[0.00062389264,0.00016624489,0.00023833325,0.00033262203,0.00045663677,0.00044097748,0.0005232827,0.00020951679,0.0002449742],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025177503,0.00009741456,0.86409044,0.00008729869,0.00018773101,0.0014386913,0.00071224355,0.060279403,0.04012211,0.008957739,0.0009742873,0.022800958],"study_design_scores_gemma":[0.000042669486,0.0001325947,0.74635756,0.000036339225,0.00007676048,0.00065243605,0.0003895151,0.23382874,0.00462235,0.011636451,0.0021891491,0.000035363315],"about_ca_topic_score_codex":0.005300544,"about_ca_topic_score_gemma":0.006645855,"teacher_disagreement_score":0.005300544,"about_ca_system_score_codex":0.00046331208,"about_ca_system_score_gemma":0.00017590837,"threshold_uncertainty_score":0.0105394125},"labels":[],"label_agreement":null},{"id":"W2890009762","doi":"10.3847/1538-4357/ab0027","title":"Cross-correlating Carbon Monoxide Line-intensity Maps with Spectroscopic and Photometric Galaxy Surveys","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Redshift; Galaxy; Complementarity (molecular biology); Grism; Carbon monoxide; Photometric redshift; Galaxy formation and evolution; Observational cosmology","score_opus":0.007085913010962819,"score_gpt":0.22038251823665583,"score_spread":0.21329660522569302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2890009762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.981309,0.0001719008,0.014715514,0.00004499337,0.000013780612,0.000019810916,0.0007052518,0.00015925874,0.0028604746],"genre_scores_gemma":[0.9951238,0.00003268358,0.00406393,0.00002257858,0.000008896914,0.0000064437622,0.0004976605,0.00001159697,0.00023237223],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988871,0.00041473962,0.00006080783,0.0002673851,0.00024594995,0.00012403152],"domain_scores_gemma":[0.99430436,0.001646457,0.001373227,0.0009972733,0.0012594247,0.00041929533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019899295,0.00024867852,0.0002522591,0.0027061251,0.0001678434,0.0009962223,0.00035155172,0.0003471475,0.00088241504],"category_scores_gemma":[0.0052459612,0.00020275425,0.00018701814,0.0018043624,0.00032711556,0.0006962194,0.0011953191,0.00021102687,0.00041442734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008175398,0.000036044705,0.9724558,0.000023030056,0.00010097156,0.000045063487,0.00009163218,0.0014688697,0.011931354,0.00058095035,0.00021614267,0.0129684685],"study_design_scores_gemma":[0.000004285867,0.00004661558,0.9858662,0.000008405433,0.000027386955,0.00011018181,0.00014292594,0.006333328,0.006175912,0.0004873633,0.0007857116,0.000011606169],"about_ca_topic_score_codex":0.0019790095,"about_ca_topic_score_gemma":0.0031298837,"teacher_disagreement_score":0.0027061251,"about_ca_system_score_codex":0.00021742085,"about_ca_system_score_gemma":0.00016088081,"threshold_uncertainty_score":0.010523915},"labels":[],"label_agreement":null},{"id":"W2890322570","doi":"10.3847/1538-4357/aad55e","title":"Formation of Nascent Product N<sub>2</sub>O from the Irradiation of O<sub>2</sub> in Icy N<sub>2</sub>","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"","keywords":"Photodissociation; Physics; Irradiation; Dissociation (chemistry); Excited state; Oxygen; Astrochemistry; Nitrogen; Photochemistry; Radiation; Nitrogen oxides; Yield (engineering); Reaction mechanism; Atomic physics; Physical chemistry; Chemistry; Interstellar medium; Astrophysics; Optics; Nuclear physics; Catalysis","score_opus":0.010218507597862565,"score_gpt":0.22464917325231537,"score_spread":0.21443066565445282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2890322570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99380517,0.0002886556,0.001785442,0.00003019656,0.00003179522,0.0000254485,0.00026930918,0.000043338932,0.0037206393],"genre_scores_gemma":[0.9952377,0.00015681777,0.0011974354,0.00004695313,0.000006326383,0.00003229732,0.000477334,0.000036045938,0.002809114],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999232,0.0000050592967,0.0000019822355,0.00002567574,0.000021983982,0.000022129732],"domain_scores_gemma":[0.9998747,0.000038649017,0.000033757402,0.000013436003,0.000020824422,0.00001858738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000107822714,0.0003533825,0.00020294324,0.00013643854,0.00024344167,0.00025967121,0.00023564979,0.00031330835,0.0027585798],"category_scores_gemma":[0.00023403026,0.00016935391,0.0001464757,0.000104839084,0.00028841555,0.00026617825,0.00023599356,0.0003548189,0.00025200885],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025348368,0.00001942966,0.0019153698,0.00005252256,0.0000076753695,0.00016977548,0.00007714318,0.00020764995,0.99550253,0.00017817022,0.00013013228,0.0014861338],"study_design_scores_gemma":[0.000022698801,0.00019830056,0.021342797,0.00000739331,0.0000120129625,0.00018371017,0.00011016195,0.0014659053,0.97442967,0.00011873194,0.0020997224,0.000008913766],"about_ca_topic_score_codex":0.002265527,"about_ca_topic_score_gemma":0.0037291292,"teacher_disagreement_score":0.0027585798,"about_ca_system_score_codex":0.0004570843,"about_ca_system_score_gemma":0.00029910973,"threshold_uncertainty_score":0.009228408},"labels":[],"label_agreement":null},{"id":"W2890375858","doi":"10.3847/1538-4357/aae822","title":"Fast and Slow Paths to Quiescence: Ages and Sizes of 400 Quiescent Galaxies from the LEGA-C Survey","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Star formation; Population; Stellar population; Peculiar galaxy; Elliptical galaxy; Galaxy formation and evolution","score_opus":0.009603377884587355,"score_gpt":0.2215019726123802,"score_spread":0.21189859472779285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2890375858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99714595,0.00019661788,0.000046047327,0.00002553276,0.0000018232802,0.000004121737,0.0020844182,0.000009633201,0.00048585466],"genre_scores_gemma":[0.9950197,0.00006263915,0.00007364335,0.000023357194,0.0000063104826,0.0000048925317,0.00456703,0.000005805732,0.00023665235],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996661,0.000060940278,0.000025523674,0.00010122158,0.000064267864,0.00008199394],"domain_scores_gemma":[0.9981974,0.0003810434,0.0005632125,0.00017417088,0.00023778019,0.00044644458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004775749,0.0002529542,0.0002593743,0.0031607042,0.00036211128,0.0009370579,0.00051450863,0.00043857057,0.0010451523],"category_scores_gemma":[0.0013431829,0.00017383066,0.00027481889,0.0016422035,0.0003518984,0.00034880204,0.000746853,0.00022282603,0.00047466604],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000745444,0.000012149302,0.9961474,0.0000099034205,0.00003808597,0.000048053207,0.00021079186,0.000056034347,0.0011152145,0.00003498597,0.00022419941,0.0020285947],"study_design_scores_gemma":[0.0000021986748,0.0000086088085,0.99935454,0.0000023178272,0.0000055425066,0.000037723352,0.000086018124,0.0000862877,0.0000744124,0.0000084323865,0.0003316517,0.0000022258314],"about_ca_topic_score_codex":0.022810712,"about_ca_topic_score_gemma":0.0299519,"teacher_disagreement_score":0.022810712,"about_ca_system_score_codex":0.0005704299,"about_ca_system_score_gemma":0.00016525364,"threshold_uncertainty_score":0.045355856},"labels":[],"label_agreement":null},{"id":"W289064884","doi":"10.1088/0004-637x/788/2/123","title":"EVIDENCE FOR ACTIVE GALACTIC NUCLEUS FEEDBACK IN THE BROAD ABSORPTION LINES AND REDDENING OF MRK 231<sup>,</sup>","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Active galactic nucleus; Spectral line; Absorption (acoustics); Absorption spectroscopy; Line (geometry); Emission spectrum; Optical depth; Galaxy","score_opus":0.02651697062399382,"score_gpt":0.2705266107328296,"score_spread":0.24400964010883575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W289064884","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972071,0.0001662632,0.00029419316,0.000089654306,0.0000059105914,0.000004269078,0.00017793401,0.000052665204,0.0020018816],"genre_scores_gemma":[0.99903417,0.000047074285,0.0002449893,0.00004419134,0.000008167789,0.0000037475045,0.00023676547,0.000010163765,0.00037077419],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994123,0.000004727666,0.000005290273,0.000017006738,0.000016385415,0.000015501004],"domain_scores_gemma":[0.9995455,0.00007914629,0.00022175862,0.000039367675,0.000043346092,0.000070812166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001051283,0.00031296324,0.00019789058,0.00021394342,0.00025578027,0.00047428202,0.00038842286,0.00033078535,0.0028496264],"category_scores_gemma":[0.0004745115,0.00017582334,0.00015845631,0.00018241825,0.0003011057,0.0002231943,0.0003589241,0.0002117349,0.000674678],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064638624,0.00014811465,0.41186002,0.0001619477,0.00008760075,0.0015563741,0.00022473716,0.0012581415,0.56718814,0.0007251129,0.00072407053,0.0154193975],"study_design_scores_gemma":[0.000014906314,0.00014097444,0.97416794,0.000007777189,0.000039953993,0.00087152614,0.00012186055,0.0018173356,0.021439347,0.00035730863,0.0010086243,0.000012450168],"about_ca_topic_score_codex":0.0022254973,"about_ca_topic_score_gemma":0.0042304527,"teacher_disagreement_score":0.0028496264,"about_ca_system_score_codex":0.0002768322,"about_ca_system_score_gemma":0.0001031564,"threshold_uncertainty_score":0.009532988},"labels":[],"label_agreement":null},{"id":"W2890876626","doi":"10.3847/1538-4357/aae38b","title":"Wide-field Optical Spectroscopy of Abell 133: A Search for Filaments Reported in X-Ray Observations","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Galaxy; Redshift; Galaxy cluster; Cluster (spacecraft); Abell 2744; Galaxy groups and clusters; Telescope; Interacting galaxy; Galaxy group","score_opus":0.024770419237583708,"score_gpt":0.2749383447175118,"score_spread":0.25016792547992805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2890876626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99825746,0.000090260575,0.00021506578,0.000035347995,0.0000027707795,0.000010682353,0.00047615494,0.000030108944,0.00088217424],"genre_scores_gemma":[0.9984308,0.000049058806,0.0005740302,0.000045495683,0.000010284314,0.000007670445,0.0006283798,0.0000091502,0.000245167],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998361,0.000013739256,0.000009380285,0.000038079714,0.000045780314,0.00005683343],"domain_scores_gemma":[0.9991242,0.000058571917,0.0004375588,0.00005193719,0.00008082091,0.0002467901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030488495,0.00025501102,0.0002593659,0.0017474124,0.0006041935,0.0006422385,0.00023286881,0.00031931954,0.0015847438],"category_scores_gemma":[0.0004044653,0.00015343168,0.00018461936,0.0012728658,0.00022549846,0.00028985285,0.00041494382,0.0003224144,0.0004394894],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020146089,0.00016108066,0.88522977,0.00003525407,0.00004946267,0.0011245044,0.0004683574,0.00007301573,0.10599377,0.00018745495,0.0008552356,0.0056207157],"study_design_scores_gemma":[0.0000018027748,0.000026874988,0.99835485,0.0000029171647,0.0000067589654,0.00023333091,0.000098208766,0.000082929815,0.00087148236,0.00001705397,0.00030118358,0.000002519535],"about_ca_topic_score_codex":0.005862006,"about_ca_topic_score_gemma":0.011978055,"teacher_disagreement_score":0.005862006,"about_ca_system_score_codex":0.00042310279,"about_ca_system_score_gemma":0.000205963,"threshold_uncertainty_score":0.011655748},"labels":[],"label_agreement":null},{"id":"W2891069754","doi":"10.3847/1538-4357/aae51c","title":"The Carnegie Supernova Project: Absolute Calibration and the Hubble Constant","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":189,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Hubble's law; Absolute (philosophy); Supernova; Astrophysics; Constant (computer programming); Calibration; Absolute magnitude; Astronomy; Cosmic distance ladder; Cosmology; Dark energy; Stars; Galaxy; Redshift; Theology","score_opus":0.012621041538781661,"score_gpt":0.2410799236283455,"score_spread":0.22845888208956383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891069754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6775461,0.0067074723,0.053297516,0.0010699672,0.0004897803,0.00063164736,0.21014407,0.0035560187,0.046557497],"genre_scores_gemma":[0.7557764,0.001369271,0.05022303,0.00025707766,0.00015810484,0.0007792034,0.18587916,0.0013704506,0.004187253],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99624157,0.0007175401,0.0002740836,0.0008283356,0.0016732535,0.0002652039],"domain_scores_gemma":[0.9856814,0.00171216,0.002674148,0.004012881,0.004907004,0.0010124316],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010203389,0.0009195974,0.00050717226,0.0072890986,0.00072097307,0.001280171,0.0012794994,0.00034278704,0.0021910542],"category_scores_gemma":[0.014925652,0.00033869242,0.00037335616,0.0066331024,0.00044092053,0.00079746253,0.0016396616,0.0007541203,0.0012498343],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054925797,0.00010332556,0.81123924,0.00031070475,0.0005436467,0.00014287798,0.00038804425,0.01310974,0.0038185501,0.014306241,0.050336674,0.10515163],"study_design_scores_gemma":[0.00003782776,0.000077081546,0.92222697,0.000104987565,0.00005285534,0.00017051112,0.00010615919,0.0070932503,0.00453818,0.0018201979,0.06370665,0.00006533483],"about_ca_topic_score_codex":0.061019532,"about_ca_topic_score_gemma":0.042273875,"teacher_disagreement_score":0.061019532,"about_ca_system_score_codex":0.0014333813,"about_ca_system_score_gemma":0.0017507444,"threshold_uncertainty_score":0.12132871},"labels":[],"label_agreement":null},{"id":"W2891121144","doi":"10.3847/1538-4357/ab01cd","title":"The NANOGrav 12.5 yr Data Set: The Frequency Dependence of Pulse Jitter in Precision Millisecond Pulsars","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Physics; Millisecond pulsar; Jitter; Pulsar; Pulse (music); Astrophysics; Millisecond; Astronomy; Optics; Detector","score_opus":0.022335029321230895,"score_gpt":0.3231983742588002,"score_spread":0.30086334493756933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891121144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928807,0.0001227107,0.0010040537,0.00005175972,0.000011269919,0.00001076822,0.0039644386,0.000093648625,0.0018606544],"genre_scores_gemma":[0.9880916,0.000051113886,0.00097035646,0.000043933265,0.000017672035,0.000019719168,0.010427774,0.000038342085,0.000339416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997143,0.000025362837,0.000027476908,0.00009346065,0.00011395012,0.000025359064],"domain_scores_gemma":[0.9981908,0.0004999213,0.0005673049,0.000407739,0.00023484085,0.00009923494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005761401,0.00016415336,0.0003103793,0.0015597749,0.00032973842,0.00037794354,0.00033864964,0.0002599157,0.0011919525],"category_scores_gemma":[0.0019302131,0.00011969442,0.0001948189,0.0015704884,0.00021965955,0.0003436874,0.00039407905,0.00029486913,0.00034925374],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052692747,0.00014260084,0.92190856,0.000106077205,0.00018926003,0.00032527364,0.0002586873,0.0056267916,0.037930712,0.00057924894,0.002958497,0.02944731],"study_design_scores_gemma":[0.000017338527,0.00004813218,0.9893967,0.0000062682298,0.000022719601,0.00018063627,0.000043375,0.00424652,0.0034507702,0.00012375669,0.0024537768,0.000009965208],"about_ca_topic_score_codex":0.0046198647,"about_ca_topic_score_gemma":0.0076192957,"teacher_disagreement_score":0.0046198647,"about_ca_system_score_codex":0.00028910048,"about_ca_system_score_gemma":0.00017048203,"threshold_uncertainty_score":0.00918597},"labels":[],"label_agreement":null},{"id":"W2891152991","doi":"10.3847/1538-4357/aad5dc","title":"Large-scale Multiconfiguration Dirac–Hartree–Fock and Relativistic Configuration Interaction Calculations of Transition Data for B-like S xii","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Configuration interaction; Hartree–Fock method; Dirac (video compression format); Scale (ratio); Atomic physics; Quantum mechanics; Excited state","score_opus":0.03349624788487041,"score_gpt":0.32575220990849485,"score_spread":0.2922559620236244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891152991","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98034704,0.0001480322,0.011501623,0.00012754419,0.000016729438,0.000025550326,0.00029985484,0.0002314199,0.0073021594],"genre_scores_gemma":[0.99512464,0.000056494726,0.0038993093,0.000022534758,0.0000063763223,0.000038849408,0.00021559974,0.000052870924,0.0005833886],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997347,0.00009726292,0.000011237782,0.000018090885,0.0000777975,0.000060888633],"domain_scores_gemma":[0.99902105,0.0005089351,0.000090728834,0.00014481015,0.00015024794,0.000084185056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009718515,0.00058745703,0.00083980756,0.0010007924,0.0014097582,0.0007533754,0.0016411697,0.000772246,0.003190491],"category_scores_gemma":[0.0013192841,0.00054301816,0.0007968746,0.0015299516,0.00084692356,0.0005168607,0.0006098249,0.00069850293,0.00029441656],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023043845,0.0001251259,0.004414785,0.00015595056,0.000074041585,0.00037954384,0.000198657,0.96389496,0.003490062,0.019480953,0.0009873926,0.006568235],"study_design_scores_gemma":[0.00008141522,0.00006218217,0.003377027,0.000016016098,0.000020804573,0.000035253986,0.000106650594,0.9907672,0.0019090277,0.0032755563,0.00032158763,0.00002729038],"about_ca_topic_score_codex":0.013198667,"about_ca_topic_score_gemma":0.01653396,"teacher_disagreement_score":0.013198667,"about_ca_system_score_codex":0.0015351146,"about_ca_system_score_gemma":0.0013673804,"threshold_uncertainty_score":0.026243687},"labels":[],"label_agreement":null},{"id":"W2891178268","doi":"10.3847/1538-4357/aafbe7","title":"The Faint End of the Centaurus A Satellite Luminosity Function","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Centaurus A; Luminosity; Luminosity function; Local Group; Galaxy; Dwarf galaxy; Satellite galaxy; Population; Surface brightness","score_opus":0.0050064384301858255,"score_gpt":0.18687550192875924,"score_spread":0.1818690634985734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891178268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97756493,0.0007033987,0.0032794257,0.0002639752,0.00004653169,0.0000064103688,0.0021538693,0.0006869338,0.015294536],"genre_scores_gemma":[0.9978295,0.00007222439,0.0005622055,0.000045129807,0.000016786871,0.0000028172014,0.00095151766,0.000027844984,0.00049203227],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982435,0.000025915897,0.000009943958,0.000056852656,0.00004957188,0.00003345499],"domain_scores_gemma":[0.9986162,0.00030878102,0.00028109632,0.00019276878,0.0002797226,0.0003214439],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036682395,0.00033307835,0.00017298193,0.002176638,0.00022658404,0.001231522,0.00030290204,0.00042520856,0.0039425823],"category_scores_gemma":[0.0017074699,0.00013345844,0.00028006354,0.00076216605,0.0004833579,0.0004812376,0.00054564833,0.00047676897,0.0016485889],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018657111,0.000030381527,0.9104275,0.00009032441,0.00010249202,0.00018692232,0.0003928774,0.0020079683,0.030971842,0.0038062069,0.0050423592,0.0467545],"study_design_scores_gemma":[0.000004131405,0.00002414913,0.99286133,0.000015850894,0.000011995457,0.00019853217,0.0000656432,0.0022296319,0.0013167926,0.000697999,0.0025664398,0.0000073192336],"about_ca_topic_score_codex":0.0035964653,"about_ca_topic_score_gemma":0.002180988,"teacher_disagreement_score":0.0039425823,"about_ca_system_score_codex":0.00039147594,"about_ca_system_score_gemma":0.00012328802,"threshold_uncertainty_score":0.013189256},"labels":[],"label_agreement":null},{"id":"W2891251091","doi":"10.3847/1538-4357/aaf37d","title":"PSR J2234+0611: A New Laboratory for Stellar Evolution","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Pulsar; Orbital inclination; Orbit (dynamics); Millisecond pulsar; Parallax; Orbital elements; Orbital eccentricity; Proper motion; Astrometry; White dwarf","score_opus":0.008800753328222626,"score_gpt":0.29732945330278243,"score_spread":0.2885286999745598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891251091","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9765802,0.0007586474,0.0065254895,0.0006903374,0.00022945245,0.00008712513,0.0003021084,0.0005969956,0.014229578],"genre_scores_gemma":[0.9916536,0.0000736493,0.005613172,0.0002598748,0.000069933005,0.000065883454,0.0005204916,0.000046672852,0.0016967399],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99926823,0.00019669146,0.000045405443,0.00019698506,0.00019169658,0.00010099292],"domain_scores_gemma":[0.9981133,0.00020720018,0.00032752875,0.0005847474,0.0002359738,0.0005312437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001852785,0.00038719122,0.00063379674,0.00079068233,0.0009395683,0.0016493032,0.00090196094,0.00077278377,0.0034684814],"category_scores_gemma":[0.0015775138,0.00018502204,0.00037446883,0.0004124848,0.00080227625,0.0008120532,0.0017007168,0.00092355977,0.0013485824],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014752602,0.0008212015,0.33652917,0.00022077849,0.000121801044,0.004299117,0.0014557261,0.0006476629,0.5123815,0.018237388,0.0055207685,0.11828965],"study_design_scores_gemma":[0.00042857302,0.005529226,0.7419963,0.0001308714,0.00018575865,0.015326627,0.0023858014,0.011841127,0.0983023,0.0141340215,0.10949313,0.00024625083],"about_ca_topic_score_codex":0.00044635427,"about_ca_topic_score_gemma":0.00073785457,"teacher_disagreement_score":0.0034684814,"about_ca_system_score_codex":0.0005092206,"about_ca_system_score_gemma":0.00040933272,"threshold_uncertainty_score":0.011603236},"labels":[],"label_agreement":null},{"id":"W2891529914","doi":"10.3847/1538-4357/aadaeb","title":"Analytical Description of the Time-dependent Perpendicular Transport of Energetic Particles","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Magnetic field; Perpendicular; Diffusion; Computational physics; Classical mechanics; Shock (circulatory); Cosmic ray; Plasma; Solar wind; Magnetohydrodynamics; Nonlinear system; Mechanics; Astrophysics; Nuclear physics; Quantum mechanics","score_opus":0.007487170372553075,"score_gpt":0.2102359380375194,"score_spread":0.2027487676649663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891529914","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.29765928,0.0025404035,0.613389,0.0016132873,0.0004293654,0.0002147085,0.00048565716,0.00045813108,0.08321017],"genre_scores_gemma":[0.9438027,0.0012875173,0.01793786,0.00017252634,0.00017750707,0.00010539326,0.00016851402,0.00010504546,0.03624303],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998847,0.000024102408,0.0000068194486,0.000021184345,0.000035362085,0.00002780909],"domain_scores_gemma":[0.999561,0.00009459519,0.00011178739,0.00003135787,0.00013612643,0.00006520762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000407328,0.0009652081,0.00045582443,0.0009982712,0.00052731705,0.0009538493,0.0010658787,0.00085809693,0.0031465478],"category_scores_gemma":[0.0014644559,0.00033071128,0.0004823996,0.00041787766,0.0011663507,0.0016715674,0.0008033679,0.0008010032,0.00050595525],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013269526,0.0001485901,0.0018894788,0.00014955169,0.00004488913,0.0011444731,0.00024243518,0.41412655,0.033409785,0.54001886,0.0021850015,0.0065077106],"study_design_scores_gemma":[0.000007726229,0.0000147286555,0.00017075938,0.000005012162,0.0000038136266,0.00007624926,0.00001722984,0.9872011,0.00040752033,0.011331123,0.000754591,0.000010223405],"about_ca_topic_score_codex":0.00525306,"about_ca_topic_score_gemma":0.0018423155,"teacher_disagreement_score":0.00525306,"about_ca_system_score_codex":0.0012054961,"about_ca_system_score_gemma":0.000688385,"threshold_uncertainty_score":0.0105262995},"labels":[],"label_agreement":null},{"id":"W2891757837","doi":"10.3847/1538-4357/aaf3bb","title":"Chemical Abundances in the Ultra-faint Dwarf Galaxies Grus I and Triangulum II: Neutron-capture Elements as a Defining Feature of the Faintest Dwarfs*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Galaxy; Metallicity; Globular cluster; Neutron star; Astronomy; Stars; Galactic halo; Halo","score_opus":0.0057968580461253685,"score_gpt":0.21434164544806222,"score_spread":0.20854478740193685,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891757837","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99944955,0.00009008217,0.000065092616,0.000004978187,0.0000011615506,0.0000012516584,0.00006334513,0.000005413571,0.00031902018],"genre_scores_gemma":[0.9993229,0.00002532862,0.00020272667,0.0000098198525,0.0000019380134,0.0000018306847,0.00028479705,0.0000035252895,0.0001471976],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999037,0.000006743066,0.000005307974,0.000035849553,0.000021988144,0.00002644558],"domain_scores_gemma":[0.999706,0.000019029854,0.00010149986,0.000022825765,0.00003589052,0.00011470638],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013417249,0.00025958038,0.00022066695,0.0011312072,0.00026891578,0.000502834,0.00035202474,0.00030767207,0.0006469943],"category_scores_gemma":[0.000322395,0.00011223999,0.00012577247,0.00045289934,0.00030828663,0.00016151916,0.00046064804,0.00016022084,0.00020882515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000159091,0.000026015512,0.8749152,0.00002348166,0.00003887191,0.00017176365,0.00029857355,0.0001330706,0.11907392,0.00018320467,0.00010383137,0.004872892],"study_design_scores_gemma":[0.0000040644745,0.000065376764,0.99388665,0.0000039325237,0.000009121315,0.00028375525,0.00018885345,0.00030689567,0.0046999888,0.00005135099,0.000495709,0.000004359085],"about_ca_topic_score_codex":0.002295591,"about_ca_topic_score_gemma":0.003147406,"teacher_disagreement_score":0.002295591,"about_ca_system_score_codex":0.00031364814,"about_ca_system_score_gemma":0.00006198946,"threshold_uncertainty_score":0.0045645237},"labels":[],"label_agreement":null},{"id":"W2891947279","doi":"10.3847/1538-4357/ab03d9","title":"Gemini GNIRS Near-infrared Spectroscopy of 50 Quasars at z ≳ 5.7","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":189,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Natural Science Foundation of China; National Science Foundation","keywords":"Physics; Quasar; Infrared; Spectroscopy; Astronomy; Astrophysics; Infrared spectroscopy; Galaxy","score_opus":0.005719978657161689,"score_gpt":0.21356008251180314,"score_spread":0.20784010385464144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891947279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992163,0.000056154044,0.00010764979,0.000009331601,0.0000013645154,0.000006216033,0.00027248348,0.000015496682,0.00031506162],"genre_scores_gemma":[0.99756986,0.000057441735,0.00052617484,0.00003505869,0.000012808296,0.000007002662,0.0014964729,0.000004633636,0.00029034962],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998153,0.00002972963,0.000011649976,0.00004334291,0.000046419027,0.000053587748],"domain_scores_gemma":[0.999613,0.000053542066,0.00011267495,0.00004144471,0.00007327341,0.00010602512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00084321626,0.00028159557,0.00021238171,0.0013216812,0.00041509868,0.0003268113,0.00022637716,0.00019013736,0.0007545437],"category_scores_gemma":[0.00042487308,0.00013772593,0.0001553979,0.00055458216,0.00019716546,0.0001898792,0.0004361007,0.00015601984,0.00025761288],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047898502,0.00018489762,0.95464784,0.000024514246,0.00007121386,0.00025117866,0.0004501908,0.00010439157,0.034037482,0.000063455416,0.00043632864,0.009249556],"study_design_scores_gemma":[0.000004083158,0.000082324295,0.99846494,8.5536396e-7,0.000014531476,0.00009224801,0.00004371268,0.000079878395,0.0009848841,0.0000053994454,0.00022569759,0.0000015619368],"about_ca_topic_score_codex":0.0026763754,"about_ca_topic_score_gemma":0.004808712,"teacher_disagreement_score":0.0026763754,"about_ca_system_score_codex":0.00020181728,"about_ca_system_score_gemma":0.00004685269,"threshold_uncertainty_score":0.0053215623},"labels":[],"label_agreement":null},{"id":"W2891952609","doi":"10.3847/1538-4357/aae20e","title":"A Deep Near-infrared [Fe ii]+[Si i] Emission Line Image of the Supernova Remnant Cassiopeia A","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Ejecta; Cassiopeia A; Supernova remnant; Supernova; Line (geometry); Emission spectrum; Mass distribution; Near-Earth supernova","score_opus":0.010600561167740007,"score_gpt":0.24078119214071703,"score_spread":0.23018063097297703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891952609","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947411,0.00017364215,0.00052279397,0.00007425325,0.000009625369,0.000010470034,0.0008424241,0.00012467222,0.0035010471],"genre_scores_gemma":[0.9952069,0.00016565902,0.0018789108,0.00004676323,0.000022417844,0.000008385441,0.0013150391,0.000020906713,0.0013350635],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999979,7.951409e-7,7.7414796e-7,0.0000067360984,0.0000046896835,0.000008095847],"domain_scores_gemma":[0.9999088,0.0000070113742,0.00001175179,0.000010350977,0.000013305733,0.000048661852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000050556362,0.00017235942,0.00010875039,0.00077063165,0.00028702887,0.0002250502,0.00016657208,0.00022901074,0.002172671],"category_scores_gemma":[0.00006425903,0.00011926785,0.00014485948,0.00026767084,0.00010564181,0.00011754681,0.00030191545,0.00030545492,0.00025063512],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053054467,0.000097988595,0.05868294,0.000097380645,0.00009170514,0.004257888,0.00024042116,0.0008844157,0.91406715,0.00024643118,0.002323552,0.018479591],"study_design_scores_gemma":[0.000020943027,0.00011890543,0.9752078,0.000020596914,0.00003667674,0.0016297954,0.00012666956,0.0017792188,0.017299186,0.00009618773,0.0036528984,0.00001098414],"about_ca_topic_score_codex":0.006775429,"about_ca_topic_score_gemma":0.010725495,"teacher_disagreement_score":0.006775429,"about_ca_system_score_codex":0.00023169965,"about_ca_system_score_gemma":0.0001387529,"threshold_uncertainty_score":0.013472021},"labels":[],"label_agreement":null},{"id":"W2891971668","doi":"10.3847/1538-4357/aae261","title":"The Reacceleration of the Shock Wave in the Radio Remnant of SN 1987A","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Supernova remnant; Physics; Astrophysics; Torus; Supernova; Telescope; Asymmetry; Brightness; Astronomy; Flux (metallurgy); Wavelength; Geometry; Optics","score_opus":0.015476750041546687,"score_gpt":0.23302688478593903,"score_spread":0.21755013474439233,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891971668","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988921,0.00017052941,0.00024428518,0.000024807303,0.000004735713,0.0000036862957,0.00013717893,0.000024950086,0.0004976303],"genre_scores_gemma":[0.9989961,0.000062545136,0.00023808348,0.000010202212,0.000009155825,0.0000031039385,0.00038023962,0.0000075340845,0.00029304408],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994445,0.000007425248,0.0000024049418,0.000009713774,0.000022012877,0.000013935306],"domain_scores_gemma":[0.99961483,0.00003972993,0.00013243171,0.0000304552,0.00010352886,0.00007904149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030250495,0.00021540755,0.00026605875,0.00066726643,0.00030835837,0.00050866144,0.00034425833,0.0002579796,0.0007337976],"category_scores_gemma":[0.0004888321,0.0001873655,0.00032168548,0.00026463368,0.00034818627,0.0001981398,0.00033538404,0.00028844964,0.00035787138],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004440372,0.00012226439,0.92082024,0.00007635023,0.00014182458,0.0026026468,0.00055765803,0.003675471,0.059359558,0.00036321912,0.0009730543,0.010863693],"study_design_scores_gemma":[0.0000056469585,0.000073006464,0.99526864,0.0000064560563,0.000021579724,0.00036202572,0.000075644144,0.0023495483,0.0010769976,0.000026203868,0.0007294999,0.000004569001],"about_ca_topic_score_codex":0.017993994,"about_ca_topic_score_gemma":0.017448965,"teacher_disagreement_score":0.017993994,"about_ca_system_score_codex":0.0005116999,"about_ca_system_score_gemma":0.00020456153,"threshold_uncertainty_score":0.035778522},"labels":[],"label_agreement":null},{"id":"W2891994652","doi":"10.3847/1538-4357/aae538","title":"Chemodynamics of Dwarf Galaxies under Ram Pressure","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; University of Southampton","keywords":"Ram pressure; Dwarf galaxy; Galaxy; Dwarf galaxy problem; Halo; Dwarf spheroidal galaxy; Tidal force; Dark matter","score_opus":0.0069749717091256574,"score_gpt":0.2171335733819977,"score_spread":0.21015860167287204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2891994652","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933183,0.000020521671,0.004534542,0.000108329834,0.0000083615905,0.000012748833,0.00012209786,0.00008548242,0.0017895276],"genre_scores_gemma":[0.9982034,0.000015812027,0.001289444,0.000024916602,0.0000031193388,0.0000125176875,0.00007169397,0.0000136274275,0.00036538375],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988556,0.000047111756,0.0000048283628,0.000018492192,0.000015829191,0.000028071898],"domain_scores_gemma":[0.99931955,0.00026812352,0.0001101016,0.000053796244,0.00009086679,0.00015761402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004785262,0.00025382196,0.00035884505,0.00049737847,0.00044374607,0.0007809258,0.00063765416,0.0004963526,0.0013742323],"category_scores_gemma":[0.0016916115,0.00024396142,0.00039581678,0.00029137894,0.0006515585,0.0004745622,0.0005684193,0.00037127075,0.00009065264],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006426952,0.00006660506,0.022236448,0.000010925782,0.00004043733,0.000114220755,0.00007450327,0.97058547,0.0014978561,0.003956643,0.0002205822,0.0011321193],"study_design_scores_gemma":[0.000023643972,0.000021797057,0.00212591,0.0000014308164,0.0000052024675,0.00000856292,0.000018472056,0.9969687,0.00012286686,0.00060407264,0.00009443259,0.0000049759365],"about_ca_topic_score_codex":0.023268841,"about_ca_topic_score_gemma":0.009971696,"teacher_disagreement_score":0.023268841,"about_ca_system_score_codex":0.0007563694,"about_ca_system_score_gemma":0.0007861647,"threshold_uncertainty_score":0.046266794},"labels":[],"label_agreement":null},{"id":"W2892181567","doi":"10.3847/1538-4357/aae151","title":"The Extraordinary Outburst in the Massive Protostellar System NGC 6334I-MM1: Flaring of the Water Masers in a North–South Bipolar Outflow Driven by MM1B","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Maser; Outflow; Bow shock (aerodynamics); Bipolar outflow; Millimeter; Radiative transfer; Excited state; Young stellar object","score_opus":0.007049013745971898,"score_gpt":0.20660772456915485,"score_spread":0.19955871082318297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2892181567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996774,0.000021708955,0.000039160877,0.00001173908,9.433871e-7,0.000001053982,0.000043822063,0.0000068382283,0.00019735724],"genre_scores_gemma":[0.9997235,0.0000141299015,0.00005536503,0.00000801302,0.000002367409,0.0000011556925,0.00009972151,0.0000018891053,0.00009393322],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999716,0.0000018148737,0.0000013542301,0.000007948928,0.0000060077928,0.000011367695],"domain_scores_gemma":[0.9998498,0.000009705974,0.000064604596,0.000011711089,0.0000105619,0.000053593987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000751514,0.0001487464,0.00015870779,0.00028352387,0.00033685967,0.00031756237,0.00015113314,0.00021459414,0.00070660724],"category_scores_gemma":[0.00017241301,0.00010088221,0.00012453408,0.00017640472,0.00016375301,0.00014047448,0.0003896761,0.000283924,0.000106572574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035331567,0.000049268423,0.7179797,0.000028669065,0.00005363774,0.0023548729,0.00061263266,0.0005137125,0.27008817,0.00016194925,0.00041720746,0.007386928],"study_design_scores_gemma":[0.0000029894607,0.000028108747,0.9978828,0.0000012414052,0.000006130197,0.00020632424,0.000081114595,0.00020881568,0.0013721751,0.00001558501,0.00019271173,0.0000019597192],"about_ca_topic_score_codex":0.0041735033,"about_ca_topic_score_gemma":0.007696379,"teacher_disagreement_score":0.0041735033,"about_ca_system_score_codex":0.0002381052,"about_ca_system_score_gemma":0.00006291409,"threshold_uncertainty_score":0.008298457},"labels":[],"label_agreement":null},{"id":"W2892555137","doi":"10.3847/1538-4357/aae847","title":"Galaxy Mergers up to Z &lt; 2.5. I. The Star Formation Properties of Merging Galaxies at Separations of 3–15 kpc","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy merger; Peculiar galaxy; Luminous infrared galaxy; Galaxy; Lenticular galaxy; Star formation; Elliptical galaxy","score_opus":0.013981763885769181,"score_gpt":0.22623052597133667,"score_spread":0.21224876208556748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2892555137","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992005,0.00013072806,0.000081424514,0.000016392072,8.859746e-7,0.000002174358,0.00017982484,0.000021613014,0.0003664804],"genre_scores_gemma":[0.99939394,0.000029786077,0.000060916715,0.0000047755448,0.000003388662,0.0000014622262,0.00040229157,0.0000040731557,0.000099319404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998266,0.000015100651,0.000008624745,0.000039972183,0.000023675822,0.000086065986],"domain_scores_gemma":[0.9987556,0.00021169598,0.00044387073,0.00007288016,0.000109323264,0.0004066771],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040894633,0.000258255,0.0003292305,0.0011049081,0.00042709368,0.00074289716,0.00026417561,0.00030149924,0.0014747165],"category_scores_gemma":[0.00091875973,0.00020470805,0.000613929,0.000895471,0.00031004837,0.0005564555,0.00056901394,0.00033540736,0.00034319414],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054063945,0.00007292718,0.96044374,0.00003074118,0.00008475497,0.00046037012,0.0003127367,0.0028202569,0.028495567,0.00036049949,0.00034195965,0.0060358695],"study_design_scores_gemma":[0.000004658463,0.00004142234,0.9966828,0.00000263766,0.000015551548,0.000069984344,0.00004646299,0.0015933292,0.0013216409,0.000043550226,0.0001741167,0.000003882785],"about_ca_topic_score_codex":0.0072705788,"about_ca_topic_score_gemma":0.005078218,"teacher_disagreement_score":0.0072705788,"about_ca_system_score_codex":0.00055573386,"about_ca_system_score_gemma":0.00020704951,"threshold_uncertainty_score":0.014456511},"labels":[],"label_agreement":null},{"id":"W2893049077","doi":"10.3847/1538-4357/ab40b2","title":"An Assessment of Contamination in the Thermal-SZ Map Using Cross-correlations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Cosmic microwave background; Physics; Astrophysics; Planck; Redshift; Weak gravitational lensing; Contamination; Astronomy; Galaxy; Anisotropy; Optics; Ecology","score_opus":0.010148035676476043,"score_gpt":0.2908306044762522,"score_spread":0.28068256879977616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2893049077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9790262,0.00024796856,0.017897507,0.00005781351,0.000018326642,0.000014854367,0.0006775299,0.00024135807,0.0018184145],"genre_scores_gemma":[0.9958733,0.000060388644,0.0025837943,0.00001950084,0.000024061455,0.0000075442154,0.0012190415,0.00006317935,0.00014913385],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9971112,0.0009124486,0.00024922343,0.000601367,0.00080267875,0.00032305814],"domain_scores_gemma":[0.97840697,0.009305893,0.00448355,0.0035745092,0.003551759,0.00067729],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005535338,0.000657459,0.00045927655,0.0035301535,0.00041312075,0.0019448422,0.0006721347,0.00042620138,0.0015824655],"category_scores_gemma":[0.019525578,0.00039891142,0.00072608364,0.0030292186,0.0008072747,0.0013152205,0.0022216665,0.00047393158,0.00033281237],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045088824,0.00005309614,0.9455731,0.00008314719,0.00099798,0.0003325215,0.00031187592,0.020490512,0.010170948,0.0027383105,0.0006195452,0.01817812],"study_design_scores_gemma":[0.000020052226,0.00009194927,0.8981389,0.00004038892,0.00024188674,0.00050122733,0.0002324437,0.08397958,0.013308259,0.0017275473,0.0016630541,0.000054745156],"about_ca_topic_score_codex":0.0039093234,"about_ca_topic_score_gemma":0.0024650828,"teacher_disagreement_score":0.005535338,"about_ca_system_score_codex":0.00046571737,"about_ca_system_score_gemma":0.00036999717,"threshold_uncertainty_score":0.029273987},"labels":[],"label_agreement":null},{"id":"W2893051096","doi":"10.3847/1538-4357/aadb95","title":"Estimating the Milky Way's Mass via Hierarchical Bayes: A Blind Test on MUGS2 Simulated Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Milky Way; Galaxy; Globular cluster; Halo; Virial theorem; Bayesian probability; Stars; Virial mass","score_opus":0.009641737889423069,"score_gpt":0.23536024428658697,"score_spread":0.2257185063971639,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2893051096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95904976,0.00011018945,0.03868049,0.00017777785,0.000022393819,0.00009538167,0.0005144042,0.0004168103,0.0009326288],"genre_scores_gemma":[0.9816636,0.000014352886,0.017193744,0.00009707551,0.000009531368,0.00004989743,0.0005901309,0.000038860187,0.00034278832],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9932648,0.0048476732,0.00017543125,0.0007967899,0.0006126946,0.00030250062],"domain_scores_gemma":[0.94566965,0.04166215,0.0029954182,0.0060970546,0.0023023423,0.0012734211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.01695211,0.0005717951,0.00073069346,0.0011716143,0.0011764679,0.001001729,0.0024711252,0.0013238423,0.0020522694],"category_scores_gemma":[0.051618136,0.00045694076,0.001100679,0.00080312253,0.0024188994,0.0009970275,0.0013117453,0.0010384851,0.00026577833],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004651929,0.00045248386,0.3586366,0.0001612398,0.0014097431,0.0004932009,0.0011604723,0.5427201,0.0058655418,0.040722918,0.004006664,0.039719094],"study_design_scores_gemma":[0.00044935656,0.0002827251,0.046476558,0.000033491237,0.00010957889,0.000094687224,0.0002249584,0.93338454,0.0060460903,0.011666326,0.0011734006,0.00005818021],"about_ca_topic_score_codex":0.03056365,"about_ca_topic_score_gemma":0.02755301,"teacher_disagreement_score":0.03056365,"about_ca_system_score_codex":0.0019290734,"about_ca_system_score_gemma":0.001429303,"threshold_uncertainty_score":0.08965242},"labels":[],"label_agreement":null},{"id":"W2893125262","doi":"10.3847/1538-4357/aadee1","title":"Unique Tracks Drive the Scatter of the Spatially Resolved Star Formation Main Sequence","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Star formation; Galaxy; Stellar mass; Accretion (finance); Galaxy formation and evolution; Range (aeronautics); Ionization; Star (game theory)","score_opus":0.010272966414375499,"score_gpt":0.22131036054553976,"score_spread":0.21103739413116426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2893125262","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985643,0.000069437905,0.00064831326,0.0000080696655,0.0000012798542,0.0000018457692,0.00027042784,0.000024110443,0.00041224138],"genre_scores_gemma":[0.9995115,0.000009824226,0.00015906552,0.0000027592441,0.0000010893916,0.0000011240284,0.0002508514,0.0000037304205,0.000060136677],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969363,0.00005760637,0.000018766188,0.00012625166,0.00006173328,0.000042151907],"domain_scores_gemma":[0.9979538,0.0005921573,0.00065610785,0.00034986675,0.00026021717,0.00018789309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005300816,0.00012165599,0.0002466986,0.001133652,0.00020916211,0.0005556335,0.00020220173,0.00020214851,0.0009342426],"category_scores_gemma":[0.0025760357,0.00015661112,0.00023309341,0.00065635686,0.00032475617,0.00023441212,0.0004408905,0.00016046516,0.00023835711],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010800634,0.0000107284695,0.980926,0.00001318521,0.00008042777,0.000042653402,0.00028288472,0.0006859479,0.012674406,0.00021198567,0.00010750352,0.0048563792],"study_design_scores_gemma":[0.0000011834572,0.000013571619,0.9979873,0.0000024540493,0.0000066282214,0.00005005991,0.000065947315,0.0009010621,0.000684699,0.000118534466,0.00016623469,0.000002455098],"about_ca_topic_score_codex":0.003100099,"about_ca_topic_score_gemma":0.0063990955,"teacher_disagreement_score":0.003100099,"about_ca_system_score_codex":0.00020901956,"about_ca_system_score_gemma":0.00011378282,"threshold_uncertainty_score":0.0061641335},"labels":[],"label_agreement":null},{"id":"W2893187301","doi":"10.3847/1538-4357/aae53a","title":"A New Generation of Cool White Dwarf Atmosphere Models. II. A DZ Star with Collision-induced Absorption","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Atmosphere (unit); Absorption (acoustics); Absorption spectroscopy; Hydrogen; Stellar atmosphere; Degeneracy (biology)","score_opus":0.020269977565169125,"score_gpt":0.22589926336775482,"score_spread":0.2056292858025857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2893187301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78675437,0.0004079092,0.19629711,0.0004775354,0.00015458997,0.00011241727,0.0019183146,0.0027523765,0.011125333],"genre_scores_gemma":[0.9400542,0.00020697417,0.05405968,0.00014589043,0.00009255574,0.00008474104,0.0013348273,0.00085964776,0.0031615132],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998714,0.000034381716,0.000009048701,0.000032588734,0.000032279546,0.0000202432],"domain_scores_gemma":[0.9995697,0.00012670062,0.000048047765,0.000091698195,0.00007708378,0.000086751475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036480857,0.0006556385,0.00048272064,0.00047264126,0.00047641507,0.0010043058,0.0010762634,0.00043824772,0.0013786335],"category_scores_gemma":[0.0015618578,0.00034327823,0.000747449,0.00028682564,0.0003358662,0.0006664552,0.001373516,0.0007931665,0.00032128734],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021884745,0.00011441984,0.03720096,0.000080244405,0.00019275959,0.00024033098,0.0002241918,0.91132164,0.010713381,0.01693529,0.002613973,0.020143963],"study_design_scores_gemma":[0.00004110126,0.000024935975,0.0013361798,0.0000043892587,0.00002019677,0.000039213188,0.000014863406,0.99265176,0.0007179253,0.0023563998,0.0027835527,0.0000095855785],"about_ca_topic_score_codex":0.010177744,"about_ca_topic_score_gemma":0.009075508,"teacher_disagreement_score":0.010177744,"about_ca_system_score_codex":0.00054945087,"about_ca_system_score_gemma":0.0005833377,"threshold_uncertainty_score":0.020236969},"labels":[],"label_agreement":null},{"id":"W2893214381","doi":"10.3847/1538-4357/aaf394","title":"A Detailed Study of the Most Relaxed SPT-selected Galaxy Clusters: Properties of the Cool Core and Central Galaxy","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Intracluster medium; Metallicity; Galaxy; Galaxy cluster; Spitzer Space Telescope; Type-cD galaxy; Spectroscopy; Inner core","score_opus":0.012392588218572522,"score_gpt":0.20191508990187806,"score_spread":0.18952250168330553,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2893214381","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994906,0.000038782087,0.0000655055,0.000007465793,4.2265947e-7,0.0000012528016,0.00013421093,0.0000040085984,0.000257705],"genre_scores_gemma":[0.99938357,0.000017533594,0.000085809814,0.000004162743,0.0000018153846,0.0000012813332,0.00037389094,0.0000028015356,0.00012912671],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990225,0.000009041907,0.0000051268094,0.000028333148,0.00002601859,0.000029223898],"domain_scores_gemma":[0.9995409,0.00005047107,0.00014231587,0.00006218417,0.00007464627,0.00012964077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015502493,0.0001625827,0.0002769167,0.001040487,0.00042135874,0.00045523452,0.0002915921,0.00014289218,0.0011912981],"category_scores_gemma":[0.00051404274,0.00012788107,0.00021650172,0.00078068656,0.0003368733,0.00022396875,0.00062952604,0.00018215268,0.00021263052],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001885512,0.000012020168,0.9623636,0.000022800614,0.00007222528,0.00014701128,0.0005295842,0.0007110164,0.031478945,0.00018699952,0.0002184116,0.0040688147],"study_design_scores_gemma":[0.0000011356625,0.000012599664,0.99921644,7.522186e-7,0.0000043429436,0.000052120122,0.000075583936,0.00023629073,0.00023618258,0.000015150023,0.00014769881,0.0000016050038],"about_ca_topic_score_codex":0.010468671,"about_ca_topic_score_gemma":0.013325261,"teacher_disagreement_score":0.010468671,"about_ca_system_score_codex":0.00026511023,"about_ca_system_score_gemma":0.00015185293,"threshold_uncertainty_score":0.020815432},"labels":[],"label_agreement":null},{"id":"W2893291898","doi":"10.3847/1538-4357/aae9df","title":"The R-Process Alliance: First Release from the Northern Search for r-process-enhanced Metal-poor Stars in the Galactic Halo","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":145,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Stars; Astrophysics; Milky Way; r-process; Galactic halo; Globular cluster; Nucleosynthesis; K-type main-sequence star; Astronomy; Halo; Galaxy; T Tauri star","score_opus":0.01714947522487298,"score_gpt":0.2698241890702283,"score_spread":0.25267471384535534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2893291898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86396915,0.0013885635,0.009347729,0.0011468406,0.00013897334,0.0010168677,0.07363187,0.0060576294,0.043302484],"genre_scores_gemma":[0.74586695,0.0005836862,0.02952597,0.00057782436,0.00026319316,0.0009945878,0.19010864,0.0025994387,0.029479723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982095,0.0003583162,0.000106553714,0.000272584,0.00080469827,0.00024853184],"domain_scores_gemma":[0.9904028,0.00081674877,0.0011629438,0.0020859414,0.0019364835,0.003595011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0075841397,0.00060216873,0.0005735825,0.0026051446,0.00056914246,0.0013257811,0.0008403747,0.0003217551,0.0033202418],"category_scores_gemma":[0.0033095963,0.0003777641,0.0005069789,0.0016917984,0.0002510879,0.00097549544,0.0031552806,0.0004130016,0.004478301],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0052174213,0.00072421174,0.7181249,0.00021309502,0.000306664,0.0006892663,0.0019958653,0.001973431,0.037095718,0.0014482156,0.05878317,0.17342812],"study_design_scores_gemma":[0.0004144143,0.0009819383,0.77396333,0.00006244404,0.000113337366,0.0005998912,0.00054611394,0.0030813976,0.009364375,0.0005199804,0.21027914,0.000073632385],"about_ca_topic_score_codex":0.0056874384,"about_ca_topic_score_gemma":0.00667192,"teacher_disagreement_score":0.0075841397,"about_ca_system_score_codex":0.0006072723,"about_ca_system_score_gemma":0.0014303031,"threshold_uncertainty_score":0.040109217},"labels":[],"label_agreement":null},{"id":"W2893846287","doi":"10.3847/1538-4357/aae43a","title":"The Complementary Roles of Feedback and Mergers in Building the Gaseous Halo and the X-Ray Corona of Milky-Way-sized Galaxies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Halo; Accretion (finance); Supernova; Galaxy; Intergalactic medium; Active galactic nucleus; Galactic halo; Galaxy formation and evolution","score_opus":0.0072638749358413,"score_gpt":0.22013408779369437,"score_spread":0.21287021285785307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2893846287","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999025,0.000056873825,0.00026558648,0.00007092739,0.000002606712,0.000002546216,0.000024414214,0.000018578083,0.0005335009],"genre_scores_gemma":[0.9996418,0.000030582018,0.00016305967,0.00001595651,0.000002478508,0.000001984537,0.000017889663,0.0000045716297,0.0001216794],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990404,0.000035702207,0.000004499427,0.000015686073,0.000010905788,0.00002913996],"domain_scores_gemma":[0.9995221,0.00014476152,0.000102136655,0.000030353094,0.000031868072,0.00016883454],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040753445,0.00038209773,0.00031220002,0.00042371347,0.0005642535,0.0010771593,0.00077037024,0.00069681054,0.0014912531],"category_scores_gemma":[0.001647642,0.0004022783,0.00057715416,0.00022094464,0.0009721418,0.0010994955,0.0010024479,0.00040750258,0.000127188],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037862305,0.0002645781,0.21157992,0.000085027576,0.00033457787,0.00062238687,0.00066609704,0.75387335,0.015549516,0.011582529,0.0004308088,0.0046326364],"study_design_scores_gemma":[0.00034653788,0.00039594443,0.16389412,0.00003189564,0.00017876543,0.00016758755,0.00071083935,0.8249088,0.0026072317,0.0056026154,0.0011058396,0.00004988563],"about_ca_topic_score_codex":0.019483034,"about_ca_topic_score_gemma":0.013457844,"teacher_disagreement_score":0.019483034,"about_ca_system_score_codex":0.0011532898,"about_ca_system_score_gemma":0.00060301786,"threshold_uncertainty_score":0.038739264},"labels":[],"label_agreement":null},{"id":"W2893985513","doi":"10.3847/1538-4357/aae487","title":"Stormy Weather in 3C 196.1: Nuclear Outbursts and Merger Events Shape the Environment of the Hybrid Radio Galaxy 3C 196.1","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Surface brightness; Active galactic nucleus; Spectral index; Galaxy; Galaxy cluster; Radio galaxy; Brightness; X-shaped radio galaxy","score_opus":0.008397641335894206,"score_gpt":0.20195848651426931,"score_spread":0.1935608451783751,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2893985513","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995047,0.000014228621,0.000020471167,0.000008784804,9.515307e-7,0.0000015039724,0.00013369172,0.000006515195,0.0003091371],"genre_scores_gemma":[0.9996,0.000009067217,0.000035869743,0.000004427487,0.0000020249338,9.812712e-7,0.0002597851,0.0000039362626,0.00008391161],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999517,0.0000036952242,0.000001732343,0.000013607778,0.000010584143,0.000018554098],"domain_scores_gemma":[0.99980956,0.00001296455,0.00007114703,0.0000110249075,0.000017927818,0.000077421464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008120672,0.000174551,0.0001843267,0.0004238472,0.00041166673,0.00056486635,0.0002073492,0.00018445784,0.0015425553],"category_scores_gemma":[0.00024953805,0.000111679714,0.00018947355,0.00046200756,0.00030495386,0.00011713505,0.0003431166,0.00024028658,0.0002930357],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007705919,0.000098890625,0.9298,0.000020990292,0.000052558094,0.0009017934,0.0005314835,0.0017371369,0.061133735,0.00027340118,0.00063169457,0.0040477235],"study_design_scores_gemma":[0.000005879345,0.000015927153,0.9987632,0.0000014200117,0.0000061765086,0.000065632725,0.00009984744,0.00054056995,0.00031960872,0.000021019472,0.0001570695,0.0000036585006],"about_ca_topic_score_codex":0.030033082,"about_ca_topic_score_gemma":0.027662966,"teacher_disagreement_score":0.030033082,"about_ca_system_score_codex":0.0005198323,"about_ca_system_score_gemma":0.00016273081,"threshold_uncertainty_score":0.059716523},"labels":[],"label_agreement":null},{"id":"W2894090759","doi":"10.3847/1538-4357/ab1a40","title":"Droplets. I. Pressure-dominated Coherent Structures in L1688 and B18","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; University of Alberta; University of Victoria","funders":"","keywords":"Lagrangian coherent structures; RADIUS; Ophiuchus; Turbulence; Velocity dispersion; Molecular cloud; Mass distribution; Magnetohydrodynamic drive","score_opus":0.005226173269705356,"score_gpt":0.2241227609805616,"score_spread":0.21889658771085624,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2894090759","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990927,0.00009497544,0.00020014126,0.000016364813,0.0000021271285,0.000008303239,0.00012564156,0.000017995306,0.00044168884],"genre_scores_gemma":[0.99907076,0.00002688844,0.0005689632,0.000008843803,0.0000053344083,0.0000049732726,0.00023199509,0.0000066158295,0.00007558343],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999411,0.0000030375188,0.000003099828,0.000015969496,0.000018453598,0.000018331497],"domain_scores_gemma":[0.99977463,0.000019460189,0.00009509475,0.000011027277,0.000022383849,0.00007742357],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007322614,0.00018056385,0.0002148781,0.0011013299,0.00037490606,0.00031842032,0.0003079547,0.0002228736,0.0009937553],"category_scores_gemma":[0.00022411978,0.00014494639,0.00013815906,0.0004460512,0.00030306267,0.00032285112,0.0005949666,0.00021777583,0.00018315934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083703804,0.00019225839,0.5216563,0.00011770814,0.000082437335,0.0028444615,0.001092021,0.0012333114,0.45106488,0.0008062293,0.0010069393,0.019066472],"study_design_scores_gemma":[0.00010483783,0.0002984186,0.9735276,0.000022363023,0.000029611336,0.0011633261,0.0005919678,0.005232522,0.015863046,0.0005446496,0.0025967367,0.00002495318],"about_ca_topic_score_codex":0.0023615225,"about_ca_topic_score_gemma":0.002086403,"teacher_disagreement_score":0.0023615225,"about_ca_system_score_codex":0.0002852086,"about_ca_system_score_gemma":0.00009107539,"threshold_uncertainty_score":0.0046955943},"labels":[],"label_agreement":null},{"id":"W2894289450","doi":"10.3847/1538-4357/aae153","title":"Extremely Dense Cores Associated with Chandra Sources in Ophiuchus A: Forming Brown Dwarfs Unveiled?","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Protostar; Outflow; Ophiuchus; Hydrostatic equilibrium; Young stellar object; Brown dwarf; Basso continuo; Star formation","score_opus":0.01517482197048521,"score_gpt":0.23190599016953373,"score_spread":0.21673116819904853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2894289450","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999426,0.0001215104,0.000081197126,0.000015219112,0.0000035433225,0.0000030224458,0.00004386033,0.0000088399975,0.0002968043],"genre_scores_gemma":[0.99978226,0.000023526583,0.0000910147,0.000005872051,0.000006462645,6.5612653e-7,0.000050064074,0.0000010579569,0.000039132243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999069,0.000008440411,0.000009846595,0.0000221496,0.000020474192,0.0000321419],"domain_scores_gemma":[0.99941707,0.00006208966,0.00022162145,0.00003558871,0.00006177762,0.00020180574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015357981,0.00017135884,0.00016606793,0.0015831618,0.00041375367,0.00058398914,0.00022256338,0.0002144859,0.0008524294],"category_scores_gemma":[0.00063245266,0.0001261074,0.00011683932,0.00048602905,0.0002880951,0.00026875638,0.00051004934,0.0001641263,0.00013976223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024199631,0.000048854796,0.9759083,0.000024394632,0.00002824984,0.0029185459,0.00026502216,0.000061664905,0.0152630545,0.00015581453,0.00017999373,0.004904175],"study_design_scores_gemma":[0.000009095781,0.00006155409,0.99177766,0.0000083725245,0.000017325243,0.0049909437,0.00037275525,0.00033065208,0.0017599756,0.00014917321,0.00051632716,0.000006185936],"about_ca_topic_score_codex":0.00233066,"about_ca_topic_score_gemma":0.0026924682,"teacher_disagreement_score":0.00233066,"about_ca_system_score_codex":0.00019836078,"about_ca_system_score_gemma":0.00017466421,"threshold_uncertainty_score":0.0046342015},"labels":[],"label_agreement":null},{"id":"W2894496257","doi":"10.3847/1538-4357/aaf97d","title":"Quiescent Galaxy Size and Spectroscopic Evolution: Combining HSC Imaging and Hectospec Spectroscopy","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; National Astronomical Observatory of Japan; Max-Planck-Gesellschaft; University of Pittsburgh; Johns Hopkins University; New Mexico State University; National Science Foundation; University of Washington; Smithsonian Institution; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; U.S. Department of Energy; York University","keywords":"Physics; Astrophysics; Stellar mass; Galaxy; Redshift; Star formation; Stellar population; Galaxy formation and evolution; Population; Astronomy","score_opus":0.0036087508884266525,"score_gpt":0.20469250298559474,"score_spread":0.20108375209716808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2894496257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974994,0.0001332413,0.0005289795,0.000028112905,0.000002644359,0.0000054926168,0.000999877,0.00006491916,0.0007373393],"genre_scores_gemma":[0.9964238,0.000046636986,0.0009703742,0.000025669124,0.000014325945,0.0000029910113,0.0023445361,0.000016665317,0.00015506039],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997011,0.000049135513,0.0000143406,0.00009914822,0.000071805785,0.000064399086],"domain_scores_gemma":[0.9986877,0.00019870859,0.00048188868,0.00017273982,0.00017662824,0.00028229313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008499244,0.00027450387,0.00028221536,0.0029667981,0.000269684,0.00087876385,0.00039435073,0.00024743262,0.0010526327],"category_scores_gemma":[0.001198133,0.00021875184,0.0003366794,0.0018132101,0.00032211238,0.0005486013,0.0008121325,0.00024309907,0.00035636267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046085108,0.00002728185,0.9895984,0.000012744476,0.000085228756,0.00005170061,0.00009721379,0.0003560089,0.003991775,0.00009407648,0.00036346779,0.0052759573],"study_design_scores_gemma":[0.0000020764592,0.000014545021,0.99797076,0.0000031438567,0.000018091421,0.000050986124,0.00007182616,0.0011572262,0.00032428064,0.00005315043,0.0003294671,0.000004532714],"about_ca_topic_score_codex":0.0054412927,"about_ca_topic_score_gemma":0.011836645,"teacher_disagreement_score":0.0054412927,"about_ca_system_score_codex":0.00026998165,"about_ca_system_score_gemma":0.00014476503,"threshold_uncertainty_score":0.010819197},"labels":[],"label_agreement":null},{"id":"W2894816434","doi":"10.3847/1538-4357/aae68e","title":"The AGN Ionization Cones of NGC 5728. I. Excitation and Nuclear Structure","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Australian Research Council; Planetary Science Division; Science Mission Directorate; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; California Institute of Technology; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Doubly ionized oxygen; Galaxy; Extinction (optical mineralogy); Active galactic nucleus; Interstellar medium; Astronomy; Ionization; Excitation; Emission spectrum; Spectral line","score_opus":0.00442018832870735,"score_gpt":0.19866314462495296,"score_spread":0.1942429562962456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2894816434","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983658,0.000052663683,0.00008160383,0.0000041529947,4.456242e-7,0.0000014763473,0.0001178952,0.00000760882,0.0013683597],"genre_scores_gemma":[0.99887854,0.000034415745,0.00013292904,0.0000026786108,0.0000011459308,0.0000026214464,0.00035323054,0.0000037184143,0.00059058506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999683,0.0000012338622,8.639315e-7,0.000009513245,0.000007437289,0.0000127662115],"domain_scores_gemma":[0.99993515,0.0000064791425,0.000023119519,0.0000050268877,0.000011052327,0.000019112033],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000027610791,0.00020480371,0.00009825519,0.0006002308,0.0001453763,0.0003073405,0.00017330701,0.000083561914,0.0010686015],"category_scores_gemma":[0.0000864524,0.00008106336,0.00009366253,0.00021035389,0.00016305559,0.00009910584,0.00026391257,0.000109679764,0.0002510867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032065995,0.0000492174,0.54967284,0.000051933435,0.000032597854,0.0014420187,0.00055001804,0.0026028878,0.42600745,0.00085168437,0.00048750674,0.017931174],"study_design_scores_gemma":[0.0000052210107,0.000038518272,0.99142754,0.000004477221,0.0000059923095,0.00043987564,0.00015891234,0.0014650384,0.0053253495,0.0001846433,0.0009395611,0.000004868007],"about_ca_topic_score_codex":0.007405011,"about_ca_topic_score_gemma":0.00626494,"teacher_disagreement_score":0.007405011,"about_ca_system_score_codex":0.00027683354,"about_ca_system_score_gemma":0.00008121966,"threshold_uncertainty_score":0.014723837},"labels":[],"label_agreement":null},{"id":"W2895146704","doi":"10.3847/1538-4357/aae690","title":"Spatially Extended Low-ionization Emission Regions (LIERs) at z ∼ 0.9","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Space Telescope Science Institute; York University; Dartmouth College; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Ionization; Astrophysics; Astronomy; Atomic physics; Ion","score_opus":0.00702204618253354,"score_gpt":0.21627416445235018,"score_spread":0.20925211826981663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2895146704","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991529,0.00004131753,0.00021704032,0.0000063636203,4.949505e-7,0.0000031339014,0.00013294665,0.00002663029,0.00041932042],"genre_scores_gemma":[0.9994217,0.00001291949,0.00024296193,0.000003632832,0.0000012109203,0.0000017695185,0.0002186863,0.0000022054548,0.000094952],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999162,0.0000050026465,0.0000046064697,0.000027061078,0.000016168959,0.000030859723],"domain_scores_gemma":[0.9996271,0.000030801704,0.00020144106,0.000026676717,0.00003435772,0.000079731566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015317324,0.00020014547,0.00015103185,0.0011687702,0.00022865421,0.00041725353,0.00024896723,0.0001500493,0.0016116519],"category_scores_gemma":[0.00031640675,0.000105704494,0.00016051582,0.0004404742,0.0001899685,0.00018845052,0.0004849214,0.00009287134,0.00032820168],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001677638,0.00003134481,0.96411186,0.00001750049,0.00002668213,0.0003741366,0.00021035773,0.00028698964,0.026490448,0.00014955043,0.00016052606,0.007972806],"study_design_scores_gemma":[0.000004803323,0.00003294402,0.99738926,0.0000031742907,0.000011453211,0.0003132702,0.00008624746,0.0005124971,0.0013114652,0.00005090202,0.0002813822,0.0000026122334],"about_ca_topic_score_codex":0.0019923388,"about_ca_topic_score_gemma":0.0028913678,"teacher_disagreement_score":0.0019923388,"about_ca_system_score_codex":0.0001581434,"about_ca_system_score_gemma":0.00007194405,"threshold_uncertainty_score":0.0053914785},"labels":[],"label_agreement":null},{"id":"W2895239141","doi":"10.3847/1538-4357/aaf6ec","title":"Eccentric Black Hole Mergers in Dense Star Clusters: The Role of Binary–Binary Encounters","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":244,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"National Research Foundation; Danmarks Grundforskningsfond; National Science Foundation","keywords":"Physics; Binary number; Astrophysics; Binary black hole; Binary star; X-ray binary; Star (game theory); Astronomy; Stars; Neutron star; Gravitational wave","score_opus":0.006552289182262758,"score_gpt":0.27029710824891195,"score_spread":0.2637448190666492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2895239141","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993368,0.00013292751,0.00010924666,0.000012975595,0.0000013248341,0.0000019083307,0.00001437716,0.0000033014878,0.00038722053],"genre_scores_gemma":[0.9998324,0.00003837699,0.00005629304,0.0000032185685,0.000002678733,6.582396e-7,0.000017840577,0.0000014218734,0.000047146823],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999749,0.00005244555,0.000008333985,0.0000770059,0.000059319646,0.00005378755],"domain_scores_gemma":[0.99861515,0.00047376586,0.0004966021,0.000106093576,0.00009261326,0.00021575266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045518484,0.0002524439,0.00027909808,0.0006310188,0.0006473671,0.0007741488,0.0003078666,0.00029076095,0.0008270658],"category_scores_gemma":[0.0016591169,0.00015451564,0.000097551354,0.00044585846,0.00080426945,0.00047310378,0.00083375606,0.00025252285,0.00010654107],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007033251,0.00014642882,0.9241249,0.00018222284,0.00018378887,0.0005551034,0.001285491,0.012695984,0.044341717,0.003972186,0.000404296,0.011404575],"study_design_scores_gemma":[0.00001620403,0.00019585715,0.97283846,0.000019592653,0.000049419195,0.00023172708,0.0006661302,0.018244138,0.0060331156,0.00095263583,0.0007308287,0.00002192378],"about_ca_topic_score_codex":0.0032719823,"about_ca_topic_score_gemma":0.0032245573,"teacher_disagreement_score":0.0032719823,"about_ca_system_score_codex":0.00041176312,"about_ca_system_score_gemma":0.00026712322,"threshold_uncertainty_score":0.0065059066},"labels":[],"label_agreement":null},{"id":"W2895335030","doi":"10.3847/1538-4357/ab09f6","title":"Revealing a Highly Dynamic Cluster Core in Abell 1664 with Chandra","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; University of Manitoba","funders":"Science and Technology Facilities Council","keywords":"Intracluster medium; Galaxy cluster; Cooling flow; Galaxy; Active galactic nucleus; Cluster (spacecraft); Luminosity; Cold front; Metallicity; Millimeter","score_opus":0.005309543949731203,"score_gpt":0.2035824563276947,"score_spread":0.1982729123779635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2895335030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99426454,0.00028013467,0.0006252641,0.00012478924,0.000025795907,0.000014209124,0.0010539048,0.00015296612,0.0034582878],"genre_scores_gemma":[0.99604046,0.00006999296,0.001623597,0.00008856617,0.00002605003,0.000008130541,0.0012305984,0.00003186725,0.00088074023],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998418,0.000008710055,0.000004905465,0.000031905027,0.000047214224,0.00006542148],"domain_scores_gemma":[0.9996629,0.000014785128,0.00008830114,0.000037059304,0.0000343754,0.00016268334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017185872,0.00034619056,0.0004091891,0.0011833778,0.0007538685,0.0007752636,0.0003829408,0.0003443537,0.0017241817],"category_scores_gemma":[0.000239704,0.00026784494,0.00032044703,0.0005157315,0.00027052584,0.00025786698,0.0008995282,0.0004021293,0.00054476154],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019324959,0.0003532743,0.39672175,0.00028141082,0.00042618363,0.005796902,0.0010245726,0.0030574296,0.55244184,0.0016593037,0.0100422725,0.02626264],"study_design_scores_gemma":[0.00002571758,0.00008816033,0.9821613,0.000014827256,0.000044755816,0.00084360456,0.00018458211,0.0018182489,0.007671038,0.0002594084,0.0068502827,0.00003807629],"about_ca_topic_score_codex":0.00904931,"about_ca_topic_score_gemma":0.018667327,"teacher_disagreement_score":0.00904931,"about_ca_system_score_codex":0.0006512881,"about_ca_system_score_gemma":0.00034156832,"threshold_uncertainty_score":0.017993271},"labels":[],"label_agreement":null},{"id":"W2895533830","doi":"10.3847/1538-4357/aaf726","title":"A Fermi Gamma-Ray Burst Monitor Search for Electromagnetic Signals Coincident with Gravitational-wave Candidates in Advanced LIGO's First Observing Run","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Industry Canada; European Regional Development Fund; Scottish Universities Physics Alliance; Bundesministerium für Bildung und Forschung; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Engineering Research Board; National Science Foundation; Science Foundation Ireland; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Russian Foundation for Basic Research; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; Kavli Foundation; National Natural Science Foundation of China; Universities Space Research Association; Royal Society; National Aeronautics and Space Administration","keywords":"Physics; Gamma-ray burst; Gravitational wave; LIGO; Kilonova; Astrophysics; Fermi Gamma-ray Space Telescope; Astronomy; Binary number; Sky; Gamma ray","score_opus":0.011923611062891774,"score_gpt":0.28846605203480224,"score_spread":0.2765424409719105,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2895533830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991062,0.000028058124,0.00017594625,0.000013459803,0.0000013943455,0.000009085463,0.00028189534,0.000026278003,0.00035749056],"genre_scores_gemma":[0.99805355,0.00002401151,0.00075793295,0.000011892784,0.000004601306,0.0000062659633,0.0008791388,0.0000066880075,0.00025574176],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975234,0.000031077805,0.000013008218,0.000061502134,0.000066057524,0.00007609536],"domain_scores_gemma":[0.9990069,0.00017267643,0.00035468768,0.00008245111,0.00008616782,0.00029707307],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005020579,0.00027449892,0.00030035223,0.0016458443,0.00046124237,0.000542792,0.0002799896,0.00026165842,0.0011261383],"category_scores_gemma":[0.0008843182,0.00013912386,0.00024486,0.000741637,0.00017212474,0.00021885907,0.0007550231,0.00022540108,0.00023167625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007785078,0.00012121394,0.9655214,0.000023272609,0.00007898841,0.0005196047,0.00028276452,0.0006297983,0.014149874,0.00015230077,0.00059189636,0.017150503],"study_design_scores_gemma":[0.000020723703,0.00023999724,0.9932221,0.0000062145787,0.000049240316,0.00030067423,0.00012982699,0.0013880096,0.0035290807,0.00006503888,0.0010391425,0.000010059609],"about_ca_topic_score_codex":0.0051817577,"about_ca_topic_score_gemma":0.0099197235,"teacher_disagreement_score":0.0051817577,"about_ca_system_score_codex":0.0003267627,"about_ca_system_score_gemma":0.00029368207,"threshold_uncertainty_score":0.010303199},"labels":[],"label_agreement":null},{"id":"W2895698080","doi":"10.3847/1538-4357/ab0f3d","title":"Search for Gravitational Waves from a Long-lived Remnant of the Binary Neutron Star Merger GW170817","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; Abdus Salam International Centre for Theoretical Physics; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; National Natural Science Foundation of China; European Commission; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; Conseil Régional, Île-de-France; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Engineering Research Board; National Science Foundation","keywords":"Neutron star; Gravitational wave; Coalescence (physics); Binary number; Detector; SIGNAL (programming language); Parameter space; LIGO; Binary star","score_opus":0.01749873801552621,"score_gpt":0.3118592782135624,"score_spread":0.2943605401980362,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2895698080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954667,0.000071385475,0.003951367,0.000034753266,0.00000403929,0.000004970392,0.000056275887,0.000064101,0.00034636402],"genre_scores_gemma":[0.99582434,0.00002361654,0.0036182324,0.000010585717,0.0000049560913,0.0000043177865,0.0003917409,0.00001698996,0.00010518039],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998474,0.00004798248,0.00000845561,0.000031964108,0.000038170678,0.000026002896],"domain_scores_gemma":[0.99868566,0.0007458934,0.00017730516,0.00009473235,0.00012260317,0.00017379587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00088760065,0.00026544736,0.00036214115,0.00069705123,0.0002985815,0.0005987153,0.00043916004,0.0004173259,0.0007373207],"category_scores_gemma":[0.0021593731,0.00016491144,0.00037334883,0.0002976538,0.00023679076,0.000354102,0.0005797471,0.00026277293,0.00017445964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0032137593,0.00051192724,0.5306999,0.00036762183,0.0014413301,0.0018705244,0.0004878449,0.16041708,0.21192342,0.0072459625,0.001412061,0.08040854],"study_design_scores_gemma":[0.00025389827,0.0011642732,0.3132313,0.00005173361,0.00041540863,0.0008573399,0.00031814678,0.6258031,0.05223325,0.0034300368,0.0021465337,0.00009501257],"about_ca_topic_score_codex":0.0010329625,"about_ca_topic_score_gemma":0.0017098085,"teacher_disagreement_score":0.0010329625,"about_ca_system_score_codex":0.00019117647,"about_ca_system_score_gemma":0.0003028296,"threshold_uncertainty_score":0.004694164},"labels":[],"label_agreement":null},{"id":"W2895918639","doi":"10.3847/1538-4357/aae695","title":"Magnetic Field Structure in Spheroidal Star-forming Clouds","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Polarization (electrochemistry); Magnetic field; Radiative transfer; SPHERES; Hourglass; Oblate spheroid; Magnetic flux; Flux (metallurgy)","score_opus":0.006704635509642275,"score_gpt":0.2317825739309382,"score_spread":0.22507793842129592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2895918639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9653278,0.00021930007,0.022470081,0.0002611734,0.000028562037,0.00004126921,0.00035345356,0.00020119539,0.011097198],"genre_scores_gemma":[0.9982503,0.000051326493,0.0006873859,0.0000136913,0.000007385001,0.000012107803,0.00007545686,0.000011464345,0.0008909482],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999349,0.000013012803,0.0000018984294,0.00001421635,0.0000139795375,0.000022047141],"domain_scores_gemma":[0.99980944,0.000035508485,0.000046285742,0.000017389993,0.00004113254,0.00005035408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014924465,0.0003229755,0.00035762243,0.00029198296,0.0006734344,0.0009777327,0.00079813617,0.00045861487,0.0009411913],"category_scores_gemma":[0.0005904194,0.00017827045,0.0002648611,0.00030525404,0.00070575596,0.00038099434,0.0003223609,0.00027491795,0.00019557006],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004562797,0.00001874811,0.004693115,0.000007264708,0.000008285565,0.000089811896,0.000043965152,0.98838633,0.001544514,0.0041945246,0.00026776848,0.0007000818],"study_design_scores_gemma":[0.000022182541,0.000017365921,0.0015926036,0.0000032513053,0.0000031125705,0.00001649141,0.000017550614,0.9965515,0.00018685979,0.0013380944,0.00024656393,0.00000434877],"about_ca_topic_score_codex":0.06508285,"about_ca_topic_score_gemma":0.01906131,"teacher_disagreement_score":0.06508285,"about_ca_system_score_codex":0.0019949044,"about_ca_system_score_gemma":0.0010578874,"threshold_uncertainty_score":0.12940806},"labels":[],"label_agreement":null},{"id":"W2896011910","doi":"10.3847/1538-4357/aae8e7","title":"The Large-scale Structure of the Halo of the Andromeda Galaxy. II. Hierarchical Structure in the Pan-Andromeda Archaeological Survey","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":180,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; McMaster University; Dalhousie University; University of Victoria; Western University; National Research Council Canada","funders":"Science and Technology Facilities Council; Canadian Space Agency; Centro de Astrofísica y Tecnologías Afines; Canadian Foundation for AIDS Research; Canarie; Centre National de la Recherche Scientifique","keywords":"Andromeda; Andromeda Galaxy; Halo; Physics; Astrophysics; Galaxy; Local Group; Astronomy; Spiral galaxy; Dwarf galaxy; Milky Way","score_opus":0.0066209298380495414,"score_gpt":0.21707136156644036,"score_spread":0.2104504317283908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896011910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971923,0.000355005,0.00064821454,0.000044541383,8.8163927e-7,0.0000056411113,0.00031134614,0.000016652695,0.0014254813],"genre_scores_gemma":[0.99873966,0.00008087367,0.00086003216,0.0000044211965,0.0000019811228,0.0000018173147,0.0001928785,0.000004738771,0.00011353089],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998636,0.000035130757,0.00000790707,0.00003457852,0.000035282144,0.000023491146],"domain_scores_gemma":[0.9993462,0.00019527433,0.00018621837,0.000098429926,0.00008828176,0.00008563214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038939854,0.00016475537,0.00010391375,0.0023401112,0.00041624662,0.00088630343,0.00024538423,0.00014413103,0.00096640526],"category_scores_gemma":[0.0010984035,0.00017492905,0.00020395406,0.0015534298,0.0006100254,0.00039027169,0.00078706944,0.00017609145,0.00021369655],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036123853,0.0000074597274,0.97487926,0.00003385951,0.00004929885,0.000075010634,0.0005962673,0.0027821998,0.0057280846,0.0016536396,0.00015235101,0.014006365],"study_design_scores_gemma":[9.988689e-7,0.0000058172204,0.9971246,0.000006027019,0.000004460456,0.000046204437,0.000289604,0.0016575332,0.0002820032,0.00025360798,0.00032416946,0.0000050659355],"about_ca_topic_score_codex":0.01818675,"about_ca_topic_score_gemma":0.04151703,"teacher_disagreement_score":0.01818675,"about_ca_system_score_codex":0.00046128916,"about_ca_system_score_gemma":0.00023654751,"threshold_uncertainty_score":0.03616178},"labels":[],"label_agreement":null},{"id":"W2896165040","doi":"10.3847/1538-4357/aaeb2d","title":"Parabolic Jets from the Spinning Black Hole in M87","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":164,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Superluminal motion; Jet (fluid); Funnel; Astrophysics; Black hole (networking); Magnetohydrodynamic drive; Magnetohydrodynamics; Very-long-baseline interferometry; Schwarzschild radius; Mechanics; Computational physics; Magnetic field; Accretion (finance)","score_opus":0.011864382090951484,"score_gpt":0.23938447305575136,"score_spread":0.2275200909647999,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896165040","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965873,0.0000782863,0.0011829371,0.00009289496,0.0000100598945,0.000009717198,0.00009342153,0.00008803217,0.0018572483],"genre_scores_gemma":[0.9992017,0.000026815007,0.00043493375,0.000024681007,0.000006422395,0.000004029298,0.000092531496,0.000013849056,0.00019510389],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99993134,0.000014819594,0.0000026777795,0.0000080973305,0.000015005527,0.00002815571],"domain_scores_gemma":[0.9997919,0.00004693891,0.00005125963,0.000021303164,0.000021992691,0.00006651479],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002018321,0.0004550599,0.00050367153,0.00028533046,0.00051397464,0.00079153344,0.0006958721,0.0005834873,0.0008681572],"category_scores_gemma":[0.00061275373,0.00019581935,0.0005246116,0.00031034704,0.00056145067,0.00028703737,0.00061209674,0.00040530652,0.00014536994],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072083203,0.00034075745,0.072639175,0.00012106407,0.00027217914,0.004722513,0.00067477283,0.86889064,0.031727813,0.009594051,0.002244686,0.008051603],"study_design_scores_gemma":[0.00017941665,0.00024482733,0.044913244,0.00001820224,0.00004630178,0.00020232679,0.00020769984,0.9480652,0.0030280575,0.0022533406,0.00080901006,0.000032433563],"about_ca_topic_score_codex":0.0075829085,"about_ca_topic_score_gemma":0.0025891303,"teacher_disagreement_score":0.0075829085,"about_ca_system_score_codex":0.00061252306,"about_ca_system_score_gemma":0.00029258485,"threshold_uncertainty_score":0.015077531},"labels":[],"label_agreement":null},{"id":"W2896222618","doi":"10.3847/1538-4357/aae983","title":"ALMA Polarimetry of Sgr A*: Probing the Accretion Flow from the Event Horizon to the Bondi Radius","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Faraday effect; RADIUS; Accretion (finance); Event horizon; Schwarzschild radius; Amplitude; Millimeter; Event (particle physics); Magnetic field; Optics","score_opus":0.01160167986483657,"score_gpt":0.23842048066542967,"score_spread":0.2268188008005931,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896222618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99325585,0.0001411106,0.0022326747,0.00004831425,0.000011332149,0.000008205149,0.0007668393,0.00009684969,0.0034387119],"genre_scores_gemma":[0.9971138,0.00006681389,0.0019229339,0.000016996328,0.000026449949,0.000007843661,0.00043194275,0.000011581902,0.0004015512],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992716,0.000013603732,0.0000029643134,0.000026821837,0.000017622277,0.000011777609],"domain_scores_gemma":[0.99983263,0.000027619726,0.00006032726,0.000019867315,0.000020849338,0.000038683156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019441289,0.00018079884,0.00012677028,0.0004522747,0.00020296258,0.00047679277,0.00013561464,0.0001718538,0.0011157214],"category_scores_gemma":[0.00025303426,0.00010557857,0.00011247419,0.00027224128,0.00013529212,0.00022828717,0.00025661662,0.0002818943,0.00033013604],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082674343,0.00009363388,0.49677587,0.000055521385,0.000086491455,0.00027861135,0.00046032073,0.0017858653,0.46841088,0.0009976157,0.0014281385,0.028800327],"study_design_scores_gemma":[0.000010025314,0.00009291067,0.9851667,0.000004748874,0.000017627992,0.00013531631,0.00007500186,0.0025368228,0.010237324,0.00014325656,0.0015736785,0.0000064917576],"about_ca_topic_score_codex":0.0010974763,"about_ca_topic_score_gemma":0.0013950504,"teacher_disagreement_score":0.0011157214,"about_ca_system_score_codex":0.00013896594,"about_ca_system_score_gemma":0.000054892516,"threshold_uncertainty_score":0.0037324429},"labels":[],"label_agreement":null},{"id":"W2896312909","doi":"10.3847/1538-4357/aaeb92","title":"The Effect of Galaxy Interactions on Molecular Gas Properties","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Star formation; Stellar mass; Control sample; Galaxy formation and evolution; Space (punctuation); Mass fraction; Plane (geometry)","score_opus":0.005886988555632005,"score_gpt":0.21788613260272677,"score_spread":0.21199914404709477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896312909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963236,0.00005730302,0.000040016777,0.0000030502222,3.9964107e-7,9.159931e-7,0.000052658026,0.0000019291783,0.00021137907],"genre_scores_gemma":[0.99985766,0.000009278419,0.000020399415,0.0000021702506,0.0000010830963,7.3534426e-7,0.00005740735,6.3247705e-7,0.000050561503],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995852,0.0001126121,0.000023466964,0.00011051289,0.000081503575,0.000086665495],"domain_scores_gemma":[0.9988562,0.00026408138,0.00043643947,0.000119617434,0.00009436204,0.00022937181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029413067,0.00021981752,0.00032472334,0.0009181521,0.00024328343,0.00047952755,0.00017753764,0.00016508308,0.0013935546],"category_scores_gemma":[0.0008121027,0.0001001995,0.00017084656,0.00050583587,0.0003867685,0.00028326776,0.0005029363,0.00015274387,0.0001673268],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014458229,0.000023112347,0.9866326,0.0000071503177,0.00006340249,0.00007417722,0.00008422246,0.000107627995,0.01085333,0.000040870385,0.000028988603,0.0019400099],"study_design_scores_gemma":[7.057972e-7,0.0000445252,0.99900466,3.5161617e-7,0.000009485605,0.000048217426,0.000038869322,0.00009687449,0.00070247264,0.000009014702,0.000043936518,9.943421e-7],"about_ca_topic_score_codex":0.0018390031,"about_ca_topic_score_gemma":0.0018463887,"teacher_disagreement_score":0.0018390031,"about_ca_system_score_codex":0.0002155976,"about_ca_system_score_gemma":0.00006537979,"threshold_uncertainty_score":0.0046619177},"labels":[],"label_agreement":null},{"id":"W2896420003","doi":"10.3847/1538-4357/aadf88","title":"Broad Wings around Hα and Hβ in the Two S-type Symbiotic Stars Z Andromedae and AG Draconis","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Balmer series; Stars; Thomson scattering; Electron density; Spectral line; Scattering; Emission spectrum; Electron temperature; Raman scattering; Doppler effect","score_opus":0.010913613553336513,"score_gpt":0.240366981191693,"score_spread":0.2294533676383565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896420003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992888,0.000051653642,0.00020251435,0.000008961081,0.0000010636387,0.0000013176716,0.000041876378,0.000013987596,0.00038974825],"genre_scores_gemma":[0.9995591,0.000017321312,0.00022964184,0.0000066375724,9.410991e-7,0.0000012655023,0.0000782002,0.000003538938,0.000103289756],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999591,0.000005365506,0.0000020658777,0.00001649892,0.000008899049,0.000008092583],"domain_scores_gemma":[0.9998704,0.000027876456,0.000037643716,0.000012329845,0.000013427632,0.00003822361],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012676604,0.00029199908,0.0001440251,0.0003514309,0.00018007332,0.0002565139,0.0002630474,0.00028487024,0.00048234325],"category_scores_gemma":[0.00021754588,0.0001609428,0.00022158006,0.00018934152,0.00016074526,0.00013632317,0.00023477738,0.00015122323,0.00014101587],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061908516,0.000091398135,0.57000726,0.0000863823,0.00019455938,0.00094647927,0.00037399153,0.021517243,0.3912575,0.00078670925,0.00026897297,0.013850462],"study_design_scores_gemma":[0.00003555092,0.00015009205,0.96257377,0.000008454906,0.000038703747,0.00037979972,0.00023434917,0.022280142,0.013365706,0.00026677203,0.0006501807,0.000016544289],"about_ca_topic_score_codex":0.0021606055,"about_ca_topic_score_gemma":0.0023628552,"teacher_disagreement_score":0.0021606055,"about_ca_system_score_codex":0.00018773119,"about_ca_system_score_gemma":0.000065645116,"threshold_uncertainty_score":0.0042960644},"labels":[],"label_agreement":null},{"id":"W2896707053","doi":"10.3847/1538-4357/aae8e1","title":"Gaps and Rings in an ALMA Survey of Disks in the Taurus Star-forming Region","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":528,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; Natural Science Foundation of Jiangsu Province; Space Telescope Science Institute; Agence Nationale de la Recherche; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Government of Jiangsu Province; National Astronomical Observatory of Japan; Koninklijke Nederlandse Akademie van Wetenschappen; European Commission; National Science Foundation; European Space Agency; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Natural Science Foundation of China; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Substructure; Planet; Protoplanetary disk; Astronomy; Spiral galaxy; Millimeter; Star formation; Galaxy","score_opus":0.027871101442049975,"score_gpt":0.2782828373530546,"score_spread":0.25041173591100463,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2896707053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99958414,0.00006130442,0.000060004524,0.0000060356947,6.692552e-7,0.0000020494429,0.00018902098,0.000005174102,0.000091496935],"genre_scores_gemma":[0.9994449,0.00003124748,0.00016823999,0.000004798844,0.0000040135633,0.000003423697,0.00027427584,0.0000012102684,0.00006787632],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996811,0.00006944613,0.000025637497,0.00009973944,0.000060743736,0.000063302134],"domain_scores_gemma":[0.9988374,0.0002001075,0.00048290778,0.0001270427,0.00015078181,0.00020177643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032984943,0.00015044672,0.00024528714,0.0017873436,0.0003487259,0.0004849614,0.00025375737,0.00026762925,0.0005077186],"category_scores_gemma":[0.0009653866,0.00014781591,0.00016273161,0.00091214513,0.0001850231,0.0003841948,0.00052583363,0.00012627659,0.00013700173],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007759659,0.000017222954,0.99277955,0.000012685779,0.000022610275,0.000062704166,0.0002479092,0.00006859895,0.0038720008,0.000020617816,0.00010013008,0.0027183017],"study_design_scores_gemma":[0.0000012926014,0.000021344173,0.9992539,0.0000018285762,0.0000057650072,0.00006840245,0.00013883271,0.00016861032,0.00017395412,0.0000075967573,0.00015745824,9.638953e-7],"about_ca_topic_score_codex":0.0035565863,"about_ca_topic_score_gemma":0.006265014,"teacher_disagreement_score":0.0035565863,"about_ca_system_score_codex":0.00017720819,"about_ca_system_score_gemma":0.00010509773,"threshold_uncertainty_score":0.0070717335},"labels":[],"label_agreement":null},{"id":"W2897048348","doi":"10.3847/1538-4357/aaeb8f","title":"Size–Luminosity Scaling Relations of Local and Distant Star-forming Regions","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Scaling; Markov chain Monte Carlo; Redshift; Galaxy; Monte Carlo method; Data set; Star formation; Luminosity; Sample (material)","score_opus":0.011034725168659077,"score_gpt":0.23886175264915785,"score_spread":0.22782702748049877,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2897048348","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99841,0.000036671834,0.0012061103,0.000010644576,2.4148247e-7,0.0000025450126,0.00014868008,0.000013731586,0.00017135624],"genre_scores_gemma":[0.9992495,0.000011566246,0.0004211113,0.0000028056274,0.000001256143,0.0000017437723,0.00028134676,0.0000036684278,0.000026944363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99942565,0.00020222846,0.000040050225,0.00017537251,0.00011551996,0.000041168583],"domain_scores_gemma":[0.98862886,0.0070718382,0.002235522,0.00094597007,0.0006602027,0.0004575791],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00252434,0.00013913022,0.00035139572,0.001411549,0.00021661198,0.0006886107,0.00044189548,0.00023595305,0.0010001004],"category_scores_gemma":[0.0135769695,0.00020740398,0.00030367266,0.0007726306,0.0005419969,0.00060578523,0.0005263122,0.00024622324,0.00014831076],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000067042696,0.000026067084,0.973932,0.0000150640435,0.00012138256,0.000057228186,0.00036706935,0.014267575,0.0031299065,0.0011555392,0.00012102066,0.0067401067],"study_design_scores_gemma":[0.000010103738,0.000041704505,0.90103656,0.000008802071,0.000033114353,0.00015542108,0.00015338184,0.09548895,0.0010118705,0.0017654707,0.00027617766,0.000018416962],"about_ca_topic_score_codex":0.0046069627,"about_ca_topic_score_gemma":0.0034209692,"teacher_disagreement_score":0.0046069627,"about_ca_system_score_codex":0.0003373247,"about_ca_system_score_gemma":0.000113130336,"threshold_uncertainty_score":0.013350189},"labels":[],"label_agreement":null},{"id":"W2897076899","doi":"10.3847/1538-4357/aae9e3","title":"The NANOGrav 11-year Data Set: Pulse Profile Variability","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"","keywords":"Pulsar; Millisecond pulsar; Physics; Astrophysics; Scintillation; Astronomy; Optics","score_opus":0.02529262294568638,"score_gpt":0.3444561926654178,"score_spread":0.3191635697197314,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2897076899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84469604,0.00058680616,0.0036045306,0.00036506873,0.00011801647,0.00007731188,0.13292216,0.0007169832,0.016913153],"genre_scores_gemma":[0.7643354,0.00024824357,0.004644367,0.0001373855,0.00006988976,0.000099650366,0.22646911,0.00025718618,0.0037387768],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995153,0.000041396226,0.000049940187,0.00011715174,0.00021544131,0.000060802216],"domain_scores_gemma":[0.99824166,0.0002822257,0.00039868322,0.00047835277,0.00045335336,0.00014571138],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007139436,0.00022331327,0.0003609166,0.0019930797,0.00038835735,0.00088831305,0.0004998256,0.00030536554,0.002850274],"category_scores_gemma":[0.0018443819,0.00012834002,0.00030472802,0.0027918464,0.00021110295,0.0005602551,0.0008294802,0.00043925212,0.0016616882],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015243576,0.00023591337,0.8223894,0.00046728752,0.00044415393,0.0009295769,0.00066290394,0.01035748,0.032930266,0.0022601432,0.042880587,0.08491787],"study_design_scores_gemma":[0.000036835107,0.00007954888,0.92941266,0.000050561455,0.00005583837,0.0003910335,0.00021323985,0.0062054237,0.0043483055,0.0004906835,0.05867312,0.000042752545],"about_ca_topic_score_codex":0.010702387,"about_ca_topic_score_gemma":0.01725204,"teacher_disagreement_score":0.010702387,"about_ca_system_score_codex":0.00045401632,"about_ca_system_score_gemma":0.00036075906,"threshold_uncertainty_score":0.02128023},"labels":[],"label_agreement":null},{"id":"W2897249401","doi":"10.3847/1538-4357/aae846","title":"KIC 2568888: To Be or Not to Be a Binary","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"Georg-August-Universität Göttingen; Centre National d’Etudes Spatiales; Belgian Federal Science Policy Office; National Aeronautics and Space Administration; California Institute of Technology; European Space Agency; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; National Science Foundation","keywords":"Red giant; Binary number; Photometry (optics); Asteroseismology; Parallax; Stars; Red-giant branch; Giant star","score_opus":0.027185510887846334,"score_gpt":0.2714424094689569,"score_spread":0.2442568985811106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2897249401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99592185,0.0000909037,0.00018157062,0.00013308894,0.000024182762,0.000006986788,0.00026821604,0.000011032329,0.003362172],"genre_scores_gemma":[0.9991394,0.000017269365,0.00011050775,0.000043162072,0.000009091502,0.0000027004583,0.00025194098,0.000004645075,0.00042133767],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997017,0.00002605754,0.00002281248,0.00008658348,0.00006851617,0.0000944203],"domain_scores_gemma":[0.9991394,0.00012941122,0.00032129747,0.000107684624,0.0001177833,0.0001843336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031970642,0.0002130699,0.00028752163,0.0009976365,0.0008290799,0.0008725163,0.00027785738,0.0006989177,0.0073384903],"category_scores_gemma":[0.0018554096,0.00010932141,0.000103560604,0.0005745753,0.00049592037,0.0003667147,0.00068000326,0.00040244093,0.0018225679],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008885278,0.00009079861,0.95340455,0.00008958609,0.000055800814,0.0038704884,0.0006353535,0.0002921747,0.022916308,0.0017205221,0.002098061,0.0139378635],"study_design_scores_gemma":[0.00006953331,0.00017134589,0.96599346,0.0001061268,0.000086900305,0.010293052,0.0027567667,0.0016555585,0.004423021,0.0037704457,0.01062993,0.00004375827],"about_ca_topic_score_codex":0.0016125444,"about_ca_topic_score_gemma":0.0023395447,"teacher_disagreement_score":0.0073384903,"about_ca_system_score_codex":0.00037763125,"about_ca_system_score_gemma":0.0001672059,"threshold_uncertainty_score":0.024549723},"labels":[],"label_agreement":null},{"id":"W2897549967","doi":"10.3847/1538-4357/ab3221","title":"Impact of Accretion Flow Dynamics on Gas-dynamical Black Hole Mass Estimates","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Supermassive black hole; Black hole (networking); Galaxy; Accretion (finance); Stellar dynamics; Stellar kinematics; Intermediate-mass black hole; Stellar mass","score_opus":0.004896209206235179,"score_gpt":0.2259493993329727,"score_spread":0.22105319012673752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2897549967","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98886275,0.00019927738,0.008651321,0.00013531794,0.0000149794505,0.00001121695,0.00031383696,0.00008215992,0.001729074],"genre_scores_gemma":[0.9991381,0.000016684742,0.00066888804,0.000008317423,0.0000031386407,0.0000011430586,0.00008600286,0.0000070298765,0.00007061535],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991295,0.0003912249,0.0000461818,0.00021097978,0.00015203464,0.00007013755],"domain_scores_gemma":[0.98868495,0.00817405,0.0016612118,0.00075921026,0.0004301184,0.00029046537],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032267957,0.00046326572,0.00030596525,0.00088023423,0.00030506,0.0013522699,0.00059447426,0.00062177965,0.0010919163],"category_scores_gemma":[0.019996198,0.00019812904,0.0002715533,0.00042725328,0.00047520362,0.0012859532,0.00093313336,0.0002849542,0.00018130448],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046843424,0.000057315847,0.8349308,0.00006026761,0.00017310446,0.00031223052,0.00018166019,0.13179943,0.0056185075,0.0057873903,0.00036651018,0.02024439],"study_design_scores_gemma":[0.00004167132,0.00022077326,0.42960057,0.00005847444,0.00007525271,0.0002518827,0.00023329648,0.54970706,0.01320744,0.0056606336,0.0008985023,0.000044367433],"about_ca_topic_score_codex":0.0051174765,"about_ca_topic_score_gemma":0.0030941349,"teacher_disagreement_score":0.0051174765,"about_ca_system_score_codex":0.0006707004,"about_ca_system_score_gemma":0.00024149375,"threshold_uncertainty_score":0.017065167},"labels":[],"label_agreement":null},{"id":"W2897755544","doi":"10.3847/1538-4357/aafd37","title":"HAWC+/SOFIA Multiwavelength Polarimetric Observations of OMC-1","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council","keywords":"Physics; Polarimetry; Polarization (electrochemistry); Astrophysics; Wavelength; Magnetic field; Ejecta; Orion Nebula; Astronomy; Star formation; Stars; Scattering; Optics; Supernova","score_opus":0.017253250640164513,"score_gpt":0.23844746285249696,"score_spread":0.22119421221233246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2897755544","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99551636,0.00007039763,0.0002470851,0.000031047402,0.000010270168,0.000011332124,0.001412188,0.00005321144,0.0026480192],"genre_scores_gemma":[0.9958054,0.000040753726,0.0012840446,0.00003210747,0.000017424527,0.000008596366,0.0023660176,0.000014506002,0.00043120483],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988806,0.000006515743,0.0000030817898,0.000034808556,0.000034122342,0.000033458844],"domain_scores_gemma":[0.99985135,0.0000076241176,0.0000416552,0.000026097654,0.000027405302,0.000045929744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022005952,0.00028530214,0.0002978633,0.00067168067,0.00036960107,0.00033425086,0.00024332377,0.00017800345,0.0008059592],"category_scores_gemma":[0.00017801244,0.00014926372,0.00018451431,0.000414891,0.00017268184,0.00015031078,0.00046719884,0.00023907337,0.00018919716],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008645234,0.00016924343,0.61558956,0.000111223344,0.00022162138,0.00065404817,0.00039225697,0.0037009816,0.32135853,0.0006229756,0.0058637955,0.050451312],"study_design_scores_gemma":[0.000024292709,0.000041610157,0.99167836,0.000006385629,0.000016611562,0.000085561405,0.00003320287,0.0017746988,0.0046437224,0.00006005965,0.0016289887,0.000006550383],"about_ca_topic_score_codex":0.0079507,"about_ca_topic_score_gemma":0.01521872,"teacher_disagreement_score":0.0079507,"about_ca_system_score_codex":0.0003856338,"about_ca_system_score_gemma":0.00024985446,"threshold_uncertainty_score":0.01580882},"labels":[],"label_agreement":null},{"id":"W2898159308","doi":"10.3847/1538-4357/ab54ce","title":"Origins of Molecular Clouds in Early-type Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Molecular cloud; Galaxy; Elliptical galaxy; RADIUS; Spiral galaxy; Galaxy cluster; Galaxy groups and clusters; Luminous infrared galaxy","score_opus":0.00547260492478258,"score_gpt":0.2105402396694975,"score_spread":0.20506763474471493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898159308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99925584,0.00024212344,0.00010865609,0.000015015195,0.0000013622781,0.0000019389352,0.000089013054,0.000011242515,0.00027497028],"genre_scores_gemma":[0.999759,0.000041321702,0.00007229355,0.000004335698,0.0000024796211,7.253007e-7,0.00007485541,0.0000019065114,0.000043035932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998092,0.000019784224,0.000007923578,0.000036941183,0.00004080244,0.00008548322],"domain_scores_gemma":[0.99842864,0.0002822958,0.00063387246,0.000130391,0.00015906255,0.00036573657],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039314321,0.0001734257,0.00028824125,0.0015078081,0.00044335367,0.0009099104,0.0003871774,0.00026864596,0.00057405554],"category_scores_gemma":[0.0012254379,0.00023303475,0.0002741262,0.0011074587,0.0005145621,0.00037222388,0.00046209892,0.00031848377,0.000107681546],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001412387,0.000023475397,0.9855108,0.000017163213,0.000041526597,0.00010655403,0.00031161142,0.0003919941,0.010123273,0.0004802954,0.00007583294,0.002776385],"study_design_scores_gemma":[0.0000031453123,0.000012550666,0.99847275,0.0000036522292,0.000009661882,0.000056150424,0.00006495983,0.00041015507,0.0006436125,0.00011182095,0.00020808743,0.000003416116],"about_ca_topic_score_codex":0.013700092,"about_ca_topic_score_gemma":0.012459447,"teacher_disagreement_score":0.013700092,"about_ca_system_score_codex":0.00076879136,"about_ca_system_score_gemma":0.00029360145,"threshold_uncertainty_score":0.027240694},"labels":[],"label_agreement":null},{"id":"W2898163744","doi":"10.3847/1538-4357/aafa01","title":"An Embedded X-Ray Source Shines through the Aspherical AT 2018cow: Revealing the Inner Workings of the Most Luminous Fast-evolving Optical Transients","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":263,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; York University","funders":"Agence Nationale de la Recherche","keywords":"Photosphere; Luminosity; Ejecta; Supernova; Spectral line; Brightness; Emission spectrum; Broadband; Shock wave","score_opus":0.008446145267561829,"score_gpt":0.22520306758587205,"score_spread":0.21675692231831023,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898163744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979988,0.00006314463,0.00014263435,0.000018679335,0.0000044988014,0.0000041579824,0.00025357964,0.000019551597,0.0014949293],"genre_scores_gemma":[0.99876165,0.000052036616,0.0002276139,0.000012117748,0.0000071906566,0.0000035776607,0.0003812721,0.000012281267,0.00054228643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996805,0.0000010124973,0.0000012310716,0.000010099076,0.000008356155,0.000011313374],"domain_scores_gemma":[0.9999027,0.0000045722827,0.00003314764,0.0000099280405,0.000016432965,0.000033221695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059927977,0.00022265803,0.00018623057,0.0006496217,0.00048724253,0.00048576918,0.00022699704,0.00023059134,0.0010867827],"category_scores_gemma":[0.00011374962,0.00012291661,0.00014777362,0.0004220858,0.00017306146,0.00023680227,0.00051194936,0.00028834268,0.0002866936],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010480919,0.00013257774,0.49862435,0.000111612375,0.00007545484,0.0058504324,0.0010219886,0.00052166916,0.4674376,0.0005259387,0.0012361924,0.023414075],"study_design_scores_gemma":[0.0000067446936,0.00008218937,0.9904303,0.000009709618,0.000017761566,0.0008310765,0.00030796233,0.00033866166,0.005645599,0.00005517365,0.0022687046,0.0000061606233],"about_ca_topic_score_codex":0.004286441,"about_ca_topic_score_gemma":0.006948933,"teacher_disagreement_score":0.004286441,"about_ca_system_score_codex":0.00027513402,"about_ca_system_score_gemma":0.00014745665,"threshold_uncertainty_score":0.008522987},"labels":[],"label_agreement":null},{"id":"W2898283427","doi":"10.3847/1538-4357/aaf21d","title":"Search for Multimessenger Sources of Gravitational Waves and High-energy Neutrinos with Advanced LIGO during Its First Observing Run, ANTARES, and IceCube","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Research, Development and Innovation Office; Institute for Global Prominent Research, Chiba University; Institut National de Physique Nucléaire et de Physique des Particules; Conselleria d'Educació, Investigació, Cultura i Esport; Labex UnivEarthS; Deutsches Elektronen-Synchrotron; Agencia Estatal de Investigación; Govern de les Illes Balears; Marsden Fund; Helmholtz Alliance for Astroparticle Physics; Istituto Nazionale di Fisica Nucleare; Conseil Régional Provence-Alpes-Côte d'Azur; RWTH Aachen University; Japan Society for the Promotion of Science; Villum Fonden; Institut Universitaire de France; Ministry of Education, India; College of Engineering, Michigan State University; Scottish Funding Council; Knut och Alice Wallenbergs Stiftelse; Industry Canada; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Conseil Régional d'Alsace; Hungarian Scientific Research Fund; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Division of Human Resource Development; Ministero dello Sviluppo Economico; Danmarks Grundforskningsfond; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Kavli Foundation; Agence Nationale de la Recherche; European Regional Development Fund; ICTP South American Institute for Fundamental Research; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; Russian Science Foundation; Office of Polar Programs; Michigan State University; Engineering and Physical Sciences Research Council; European Commission; Leverhulme Trust; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Science and Engineering Research Board; Polarforskningssekretariatet; National Natural Science Foundation of China; Scottish Universities Physics Alliance; National Research Foundation of Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Australian Research Council; Western Canada Research Grid; Natural Sciences and Engineering Research Council of Canada; Ministerio de Economía y Competitividad; Bundesministerium für Bildung und Forschung; Institut des Origines de Lyon; Canadian Institute for Advanced Research; Autoritatea Natională pentru Cercetare Stiintifică; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; Chiba University; Royal Society; Belgian Federal Science Policy Office; National Science Foundation; Compute Canada; Marquette University; Abdus Salam International Centre for Theoretical Physics","keywords":"LIGO; Neutrino; Gravitational wave; Neutron star; Binary number; Binary black hole; Solar neutrino problem; Gravitational-wave astronomy; Gravitational-wave observatory","score_opus":0.008705465076731844,"score_gpt":0.2615391283535415,"score_spread":0.2528336632768096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898283427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99709225,0.00009302539,0.0003640836,0.00004544951,0.0000058826213,0.000015234949,0.0013761806,0.000028023684,0.0009799214],"genre_scores_gemma":[0.9950864,0.0000712441,0.001071639,0.000022695753,0.000017587277,0.000024610597,0.0032993841,0.000017513798,0.0003890102],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995596,0.00006960728,0.000026164238,0.00015051886,0.0001068995,0.0000871758],"domain_scores_gemma":[0.9981021,0.0004670955,0.00085628906,0.0001720498,0.0001365208,0.0002659139],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009832648,0.0003159064,0.00042616136,0.0015456415,0.00060097955,0.0010467601,0.0003345059,0.000350393,0.001104343],"category_scores_gemma":[0.0014683855,0.00022554706,0.0003026968,0.0012010712,0.00027098224,0.00037914468,0.0008851856,0.00039202586,0.00017747909],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038387702,0.000062628176,0.9852985,0.000023708893,0.00012261709,0.00014056177,0.00024478638,0.000560691,0.0064520272,0.00028565744,0.00036168855,0.0060632722],"study_design_scores_gemma":[0.000021599726,0.00004518208,0.99599636,0.000007962762,0.000035705307,0.000087951776,0.000085917236,0.0011665387,0.0012862202,0.00010293181,0.0011569017,0.000006614393],"about_ca_topic_score_codex":0.008262946,"about_ca_topic_score_gemma":0.016264455,"teacher_disagreement_score":0.008262946,"about_ca_system_score_codex":0.00046263024,"about_ca_system_score_gemma":0.00039387489,"threshold_uncertainty_score":0.016429663},"labels":[],"label_agreement":null},{"id":"W2898444044","doi":"10.3847/1538-4357/ab01ca","title":"Mass Calibration of Optically Selected DES Clusters Using a Measurement of CMB-cluster Lensing with SPTpol Data","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; Canadian Institute for Advanced Research","funders":"Science and Technology Facilities Council; Office of Science; National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Cosmic microwave background; Physics; Weak gravitational lensing; Astrophysics; Galaxy cluster; Gravitational lens; Galaxy; Estimator; Redshift; Anisotropy; Statistics; Optics; Mathematics","score_opus":0.02288956417068633,"score_gpt":0.2219532832688949,"score_spread":0.19906371909820858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898444044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941848,0.000059539765,0.002631422,0.000029841925,0.0000044311755,0.000013335434,0.0011344133,0.00011773739,0.0018245362],"genre_scores_gemma":[0.9937966,0.0000343476,0.0026919688,0.00002049116,0.000011205006,0.000015896723,0.0031842575,0.000043213335,0.00020201108],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992084,0.00014622769,0.000033000328,0.00025615198,0.00026901084,0.00008728657],"domain_scores_gemma":[0.9980258,0.00035626497,0.00066417694,0.00040616337,0.0003529643,0.00019457827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010388072,0.00052195165,0.00029899227,0.0025843778,0.00032402013,0.000708655,0.00065380434,0.0002701135,0.0013312941],"category_scores_gemma":[0.0033903248,0.0003329155,0.00025752865,0.001951161,0.00035193027,0.0005330975,0.0011147106,0.00032010686,0.0005593749],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025764425,0.00005521631,0.95550394,0.0000346746,0.00018518137,0.00012852131,0.00024086049,0.012888917,0.013527921,0.0011384973,0.0014301323,0.014608476],"study_design_scores_gemma":[0.000020767144,0.000040057294,0.96687216,0.000009307894,0.000024893945,0.000084292835,0.00010420754,0.024812188,0.0060124113,0.00039673518,0.0016054334,0.000017479486],"about_ca_topic_score_codex":0.008330533,"about_ca_topic_score_gemma":0.01089418,"teacher_disagreement_score":0.008330533,"about_ca_system_score_codex":0.0008641594,"about_ca_system_score_gemma":0.00021851023,"threshold_uncertainty_score":0.016564071},"labels":[],"label_agreement":null},{"id":"W2898479862","doi":"10.3847/1538-4357/aaecd1","title":"Forming Super Star Clusters in the Central Starburst of NGC 253","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Western University","funders":"Astrophysics Division; National Astronomical Observatory of Japan; National Science Council; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Star cluster; Star (game theory); Hubble sequence; Astronomy; Galaxy; Luminous infrared galaxy","score_opus":0.011618313250527165,"score_gpt":0.22771988747528174,"score_spread":0.21610157422475457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898479862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953616,0.000022497356,0.00004389509,0.000009646002,0.0000016209422,0.00000184534,0.000052836054,0.000006339598,0.00032521793],"genre_scores_gemma":[0.99967206,0.000015257058,0.000057365058,0.000006552679,0.0000023090993,0.0000015798012,0.00012474015,0.0000015489674,0.000118658165],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993765,0.0000049762734,0.000004757695,0.000021488533,0.000011310258,0.000019787898],"domain_scores_gemma":[0.9996772,0.000020895379,0.000114157105,0.00002526984,0.00002780462,0.00013476341],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001168742,0.00015470377,0.00019100904,0.00036549542,0.00050452875,0.00043568164,0.00020959332,0.00016173722,0.0017733807],"category_scores_gemma":[0.0002444772,0.00013480046,0.00014812166,0.00026327622,0.0002340992,0.00011331495,0.0003124442,0.00017256662,0.00031446764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014601822,0.000055304525,0.972376,0.0000072198527,0.000029342476,0.0013007968,0.0002925492,0.00023753688,0.022484103,0.00015173563,0.00026596067,0.0026535213],"study_design_scores_gemma":[0.0000036324655,0.000030320283,0.9984426,0.000002226266,0.0000072490857,0.0004452541,0.0001995165,0.0002490049,0.0003775512,0.000048031958,0.00019262153,0.000002185927],"about_ca_topic_score_codex":0.014301145,"about_ca_topic_score_gemma":0.02363027,"teacher_disagreement_score":0.014301145,"about_ca_system_score_codex":0.00038928067,"about_ca_system_score_gemma":0.00020626961,"threshold_uncertainty_score":0.028435826},"labels":[],"label_agreement":null},{"id":"W2898683405","doi":"10.3847/1538-4357/ab3426","title":"Pulsational Pair-instability Supernovae in Very Close Binaries","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":200,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Astrophysics Division; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; National Science Foundation","keywords":"Roche lobe; Supernova; Binary number; Binary black hole; Binary star; Stars; Helium; Stellar evolution; Neutron star","score_opus":0.009566831548341082,"score_gpt":0.22457686514729722,"score_spread":0.21501003359895612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898683405","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99879104,0.000043928507,0.0006650019,0.0000071338673,0.0000021140954,0.000002427019,0.00003559268,0.000012311132,0.00044044727],"genre_scores_gemma":[0.9996728,0.000011575327,0.00015948404,0.0000028344737,0.0000017930688,0.000001547011,0.0000780361,0.0000025046988,0.000069477675],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991477,0.000019063149,0.000005291525,0.000020969464,0.000021902748,0.00001800994],"domain_scores_gemma":[0.99969006,0.000118518365,0.00007696803,0.000025315318,0.000017193177,0.00007202666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021049254,0.0001903017,0.00032416006,0.00041674968,0.00033458148,0.0005978275,0.00027362694,0.00026995773,0.0011285245],"category_scores_gemma":[0.0007894254,0.00016828618,0.00029067532,0.0003811849,0.00031179225,0.00027021472,0.00061182556,0.00024696736,0.00011698659],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041679115,0.00024450338,0.7196684,0.00007116326,0.00030789178,0.0014416967,0.00016214416,0.24088731,0.025121216,0.0045397785,0.00032719853,0.006811951],"study_design_scores_gemma":[0.000067004265,0.00038932968,0.47946334,0.000014230675,0.000061772036,0.0010797328,0.00020461815,0.5062439,0.008308742,0.0030926708,0.0010388512,0.000035861445],"about_ca_topic_score_codex":0.0017343427,"about_ca_topic_score_gemma":0.0012513441,"teacher_disagreement_score":0.0017343427,"about_ca_system_score_codex":0.0003550654,"about_ca_system_score_gemma":0.00011905026,"threshold_uncertainty_score":0.0037752986},"labels":[],"label_agreement":null},{"id":"W2898696636","doi":"10.3847/1538-4357/aaee7b","title":"Hunting for Radio Emission from the Intermittent Pulsar J1107-5907 at Low Frequencies","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Pulsar; Physics; Radio telescope; Astrophysics; Low frequency; Pulse (music); Spectral index; Astronomy; Optics; Spectral line; Detector","score_opus":0.017264216936613605,"score_gpt":0.3103817448656862,"score_spread":0.2931175279290726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898696636","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978035,0.000087128195,0.0009467508,0.000038754268,0.0000074954955,0.0000032076782,0.00011176103,0.000030946165,0.0009705338],"genre_scores_gemma":[0.9981541,0.00004836304,0.0010923212,0.000036474077,0.000018325369,0.0000057906136,0.00042418586,0.000011236784,0.00020920696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991214,0.000009614486,0.000003755408,0.000027104774,0.000024995104,0.000022254908],"domain_scores_gemma":[0.9995485,0.00011868583,0.00013747015,0.000049386985,0.000059170412,0.00008666199],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019588153,0.000110876135,0.00028803851,0.0006135675,0.00030788247,0.00051035546,0.00023903302,0.0002952686,0.00079221145],"category_scores_gemma":[0.00050864764,0.00014646954,0.00013711426,0.0004390736,0.00028144312,0.0002250019,0.00037300432,0.00034959702,0.0003436009],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016536313,0.000084659536,0.7848733,0.00006303326,0.000101336766,0.0008067687,0.0003954025,0.0005393572,0.18611117,0.00055120996,0.001280571,0.025027772],"study_design_scores_gemma":[0.0000067188616,0.00009640984,0.9915542,0.000013176211,0.000032552678,0.0006690714,0.00019218825,0.0017201606,0.004135605,0.00026051124,0.0013102989,0.000009051525],"about_ca_topic_score_codex":0.00064964156,"about_ca_topic_score_gemma":0.0017794899,"teacher_disagreement_score":0.00079221145,"about_ca_system_score_codex":0.00017141081,"about_ca_system_score_gemma":0.000085371736,"threshold_uncertainty_score":0.0026502013},"labels":[],"label_agreement":null},{"id":"W2898744282","doi":"10.3847/1538-4357/aafda3","title":"Impulsive Electromagnetic Emission near a Black Hole","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Polarization (electrochemistry); Gravitational wave; Supermassive black hole; Gravitational lens; Black hole (networking); Spin-flip; Electromagnetic pulse; Gravitation; Electromagnetic radiation; Accretion (finance)","score_opus":0.005471459840478171,"score_gpt":0.2818727172012102,"score_spread":0.27640125736073207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898744282","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99643815,0.00005905473,0.0019225142,0.000013866472,0.0000036331714,0.000003341214,0.000026566066,0.00005381442,0.001479022],"genre_scores_gemma":[0.99934095,0.000018714414,0.00037956153,0.000004239321,0.0000057881684,0.0000010507955,0.000033627046,0.000004413863,0.0002116357],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999658,0.0000051330503,0.0000010232906,0.000007924812,0.000012050533,0.000008012724],"domain_scores_gemma":[0.9998536,0.00004680952,0.000040661103,0.000015368942,0.000013415541,0.00003010031],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009913212,0.00017817512,0.00017608037,0.00036918133,0.00014270144,0.00024589148,0.0001578957,0.00021714675,0.00090267754],"category_scores_gemma":[0.0002772784,0.00007401439,0.00012440057,0.00022087975,0.00017895254,0.000120328856,0.00031232327,0.00018842483,0.00010804668],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009523021,0.000110837005,0.10069534,0.00011600773,0.00011243329,0.006084753,0.00043080215,0.0115640685,0.84117645,0.0042525157,0.00044541553,0.03405908],"study_design_scores_gemma":[0.00009367025,0.0013425977,0.80789334,0.000028889594,0.00008165258,0.004102284,0.00031857073,0.0548869,0.1250758,0.003680118,0.0024327897,0.00006340658],"about_ca_topic_score_codex":0.0002496173,"about_ca_topic_score_gemma":0.00015596228,"teacher_disagreement_score":0.00090267754,"about_ca_system_score_codex":0.00014635926,"about_ca_system_score_gemma":0.000034807592,"threshold_uncertainty_score":0.0030197501},"labels":[],"label_agreement":null},{"id":"W2898775218","doi":"10.3847/1538-4357/ab1846","title":"ALMA Reveals Potential Evidence for Spiral Arms, Bars, and Rings in High-redshift Submillimeter Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":143,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Korea Astronomy and Space Science Institute; National Science Foundation; Ministerio de Economía y Competitividad; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Council; National Radio Astronomy Observatory","keywords":"Galaxy; Spiral galaxy; Star formation; Submillimeter Array; Luminous infrared galaxy; Elliptical galaxy; Angular momentum; Curvature; Extinction (optical mineralogy)","score_opus":0.011930420124729904,"score_gpt":0.23197588721080267,"score_spread":0.22004546708607275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2898775218","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993643,0.00002865526,0.00014383433,0.000009453828,7.864555e-7,0.0000011213982,0.00005395851,0.000019128447,0.0003786779],"genre_scores_gemma":[0.9996456,0.000007249408,0.00018302632,0.000007407959,0.000002460346,9.610928e-7,0.000068640045,0.0000015875221,0.00008302279],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999236,0.000008443522,0.0000037340806,0.000020160853,0.000017066392,0.00002701739],"domain_scores_gemma":[0.9995741,0.000074382544,0.0001432016,0.00006530032,0.000041031744,0.000102014645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001859848,0.00014452312,0.00013071744,0.00074996654,0.00018362814,0.00047586992,0.0002113674,0.00019204266,0.0013668056],"category_scores_gemma":[0.00036110778,0.000110976085,0.00016102032,0.00027986363,0.00024943933,0.00019658898,0.00031517327,0.00016672541,0.00028788205],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000948297,0.000040350536,0.93536776,0.000017755245,0.000034128992,0.00014681811,0.0002944729,0.00027955667,0.056278307,0.00018330678,0.0001473881,0.007115291],"study_design_scores_gemma":[0.000001981686,0.000027632013,0.99820566,0.000001695569,0.0000059294166,0.00008866115,0.00006509108,0.0003298116,0.0010651837,0.00003607064,0.00017061402,0.0000016070942],"about_ca_topic_score_codex":0.0015081342,"about_ca_topic_score_gemma":0.0029700284,"teacher_disagreement_score":0.0015081342,"about_ca_system_score_codex":0.00016093327,"about_ca_system_score_gemma":0.000056812532,"threshold_uncertainty_score":0.0045723915},"labels":[],"label_agreement":null},{"id":"W2899492310","doi":"10.3847/1538-4357/aaf1bf","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Systematic Investigations of Short-timescale C IV Broad Absorption Line Variability","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Quasar; Sky; Reverberation mapping; Spectral line; Epoch (astronomy); Outflow; Line (geometry); Spectral slope","score_opus":0.014801982519407023,"score_gpt":0.22540277255681235,"score_spread":0.21060079003740534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2899492310","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968064,0.0002194592,0.0005395031,0.000022848682,0.0000017576116,0.000014560119,0.0020320937,0.000017249427,0.00034614545],"genre_scores_gemma":[0.9928042,0.00020041465,0.0012989001,0.000025875881,0.0000073902124,0.00003594662,0.0054245135,0.000015495107,0.00018728041],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989447,0.00042027264,0.00007423851,0.00019785968,0.0002500172,0.00011292062],"domain_scores_gemma":[0.9947525,0.0012432063,0.0021195705,0.0007757068,0.0006317157,0.0004773181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023312676,0.00029071217,0.00022326391,0.003374633,0.00035316648,0.0005654034,0.0004486745,0.00019183147,0.0003948953],"category_scores_gemma":[0.003333214,0.00016693509,0.00037373824,0.0027001773,0.00033258842,0.00040928333,0.0009473487,0.00019651758,0.0001835548],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003790326,0.00002925693,0.9887135,0.000031772546,0.00011672365,0.00008994622,0.00026713367,0.00024385509,0.001930788,0.000045185207,0.00032771254,0.008166354],"study_design_scores_gemma":[0.0000017985633,0.000021030071,0.99864,0.0000051739594,0.000014771732,0.00007009937,0.000113480164,0.00024614693,0.00030707952,0.000009696975,0.0005673722,0.0000033381677],"about_ca_topic_score_codex":0.01397336,"about_ca_topic_score_gemma":0.025479002,"teacher_disagreement_score":0.01397336,"about_ca_system_score_codex":0.00026104244,"about_ca_system_score_gemma":0.00047844704,"threshold_uncertainty_score":0.02778405},"labels":[],"label_agreement":null},{"id":"W2899540813","doi":"10.3847/1538-4357/aaee8b","title":"Testing Feedback-regulated Star Formation in Gas-rich, Turbulent Disk Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Star formation; Galaxy; Dynamo; Hydrostatic equilibrium; Ram pressure; Galaxy formation and evolution; Velocity dispersion; Luminous infrared galaxy; Turbulence; COSMIC cancer database","score_opus":0.010789327562037267,"score_gpt":0.22004544269073215,"score_spread":0.20925611512869488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2899540813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99976,0.000012189838,0.00009112313,0.0000025559746,3.8628514e-7,9.622576e-7,0.000026367215,0.000004341292,0.00010209007],"genre_scores_gemma":[0.99991524,0.0000030807391,0.00003249284,0.0000014916375,4.944442e-7,7.6801086e-7,0.000028213259,5.2602695e-7,0.000017724711],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981505,0.000050866845,0.000011091596,0.000045091925,0.00003909518,0.000038882237],"domain_scores_gemma":[0.99834156,0.0006629449,0.00046378974,0.00012276623,0.000134107,0.00027481516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039909303,0.00018583641,0.00016240607,0.00046748266,0.00016598165,0.00040421396,0.00020119784,0.00015310885,0.0007383635],"category_scores_gemma":[0.0017979556,0.000085229876,0.00016199931,0.00025824909,0.00031163264,0.00025380187,0.00033330166,0.00011778029,0.00009696439],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000111909976,0.000041495918,0.9841855,0.000011286662,0.000040876937,0.000043048145,0.0001346513,0.0006054263,0.011745913,0.00008768046,0.000025021242,0.002967144],"study_design_scores_gemma":[0.000003825464,0.000106601845,0.9954997,0.000001461702,0.000011188939,0.000040193172,0.00009644719,0.0017257829,0.002401822,0.000047742225,0.000062775485,0.0000023713778],"about_ca_topic_score_codex":0.0023679142,"about_ca_topic_score_gemma":0.0026777403,"teacher_disagreement_score":0.0023679142,"about_ca_system_score_codex":0.00028151076,"about_ca_system_score_gemma":0.00013335234,"threshold_uncertainty_score":0.00470829},"labels":[],"label_agreement":null},{"id":"W2899580011","doi":"10.3847/1538-4357/aaeff5","title":"ALMA Detections of the Youngest Protostars in Ophiuchus","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics; Western University","funders":"National Institutes of Natural Sciences; National Astronomical Observatory of Japan; National Science Council; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Canadian Institute for Theoretical Astrophysics; National Radio Astronomy Observatory; National Science Foundation","keywords":"Ophiuchus; Physics; Astrophysics; Protostar; Bipolar outflow; Molecular cloud; Submillimeter Array; Millimeter; Outflow; Astronomy; Accretion (finance); Star formation; Stars","score_opus":0.010546100656756754,"score_gpt":0.24294219861691993,"score_spread":0.23239609796016317,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2899580011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994,0.000030103303,0.00006069429,0.000006315172,0.0000011073693,0.0000014786845,0.000074796146,0.000009519361,0.00041601394],"genre_scores_gemma":[0.9994698,0.000013258327,0.00020623933,0.000007686529,0.00000402039,0.0000017262468,0.00016730018,0.0000016761206,0.00012827339],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993,0.00000550504,0.000004763061,0.000020288628,0.000024617044,0.000014738068],"domain_scores_gemma":[0.99967563,0.000035198627,0.00010802566,0.000027136637,0.000037750873,0.000116342664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013569057,0.00011025945,0.00013073625,0.00066875684,0.0003388754,0.00029001178,0.00018482827,0.0001866177,0.0008284414],"category_scores_gemma":[0.00029780623,0.00010408482,0.0000891711,0.00024390468,0.00017104116,0.00016740483,0.00043327757,0.00014906317,0.00012522427],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017952289,0.000049776267,0.8987183,0.000025672842,0.00003301133,0.00031296525,0.00054885953,0.0002260763,0.089019634,0.00013797406,0.000268473,0.010479684],"study_design_scores_gemma":[0.0000036826839,0.000027390399,0.99796957,0.0000022364145,0.0000041158128,0.00010571543,0.00006514783,0.0002599926,0.0012625059,0.00002197944,0.00027616034,0.000001502532],"about_ca_topic_score_codex":0.0024653045,"about_ca_topic_score_gemma":0.006205443,"teacher_disagreement_score":0.0024653045,"about_ca_system_score_codex":0.00024135955,"about_ca_system_score_gemma":0.00007935931,"threshold_uncertainty_score":0.0049019456},"labels":[],"label_agreement":null},{"id":"W2899833098","doi":"10.3847/1538-4357/ab14f3","title":"Revisiting the Size–Luminosity Relation in the Era of Ultra Diffuse Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Coma Cluster; Elliptical galaxy; Galaxy; Brightest cluster galaxy; Surface brightness; Halo; Peculiar galaxy; Luminous infrared galaxy; Surface brightness fluctuation; Galaxy cluster","score_opus":0.006398015152539423,"score_gpt":0.20663524063487446,"score_spread":0.20023722548233502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2899833098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948114,0.000798936,0.00060927344,0.00041115467,0.0000043410682,0.000002041872,0.0001232193,0.000011535561,0.0032280132],"genre_scores_gemma":[0.9993748,0.000117244235,0.00017622397,0.000052039122,0.000013135272,7.8701595e-7,0.000053520784,0.0000042268566,0.00020817455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972266,0.00005692923,0.000010654638,0.00009565381,0.0000656773,0.00004850209],"domain_scores_gemma":[0.9963276,0.0015435755,0.0010014524,0.0003371487,0.00040165093,0.00038850453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00090063934,0.00010128367,0.00021723848,0.0017125681,0.0004994529,0.0013989566,0.0005221484,0.00035706337,0.0021719444],"category_scores_gemma":[0.0039332095,0.00018454596,0.00012230164,0.001423963,0.0013218946,0.0014921011,0.001095113,0.00045960833,0.00022524598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008450123,0.000029154897,0.9608048,0.000029283161,0.000024463685,0.00015081797,0.0017673933,0.00036328158,0.0054121786,0.008592436,0.00074397796,0.021997662],"study_design_scores_gemma":[0.0000022559743,0.000016797765,0.9946128,0.000009107762,0.0000071339514,0.00012035927,0.00046082048,0.0004684192,0.0003194815,0.0012812428,0.0026969714,0.0000046407167],"about_ca_topic_score_codex":0.0070069795,"about_ca_topic_score_gemma":0.013844047,"teacher_disagreement_score":0.0070069795,"about_ca_system_score_codex":0.0006846077,"about_ca_system_score_gemma":0.00023152654,"threshold_uncertainty_score":0.013932347},"labels":[],"label_agreement":null},{"id":"W2900266151","doi":"10.3847/1538-4357/aaee7a","title":"Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). V. Quasar Luminosity Function and Contribution to Cosmic Reionization at z = 6","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":223,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Quasar; Reionization; Luminosity function; OVV quasar; Sky; Luminosity; Galaxy; Flattening; Intergalactic travel","score_opus":0.00913580182122649,"score_gpt":0.21101045771886798,"score_spread":0.20187465589764148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2900266151","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948919,0.00023869556,0.0009965792,0.000038148624,0.0000030725,0.0000068799245,0.0012535172,0.00007500417,0.0024962262],"genre_scores_gemma":[0.9967452,0.00009779753,0.00088338304,0.000016582595,0.00001236019,0.0000052709,0.0015760205,0.000015080075,0.0006482672],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982303,0.000037602145,0.000009518578,0.000034544682,0.00006036271,0.000035013803],"domain_scores_gemma":[0.9987167,0.00020039288,0.0005086501,0.00016076028,0.00020146558,0.00021205469],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005956349,0.00023761309,0.00016922606,0.0019425665,0.00018728706,0.00057463965,0.00019395056,0.00012858758,0.0010719002],"category_scores_gemma":[0.00086520164,0.00008835497,0.00022944676,0.00062721106,0.00019951501,0.00042041988,0.0006703068,0.00018756102,0.00036640474],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010292549,0.000021346608,0.9707809,0.00002258161,0.00003087941,0.000064953616,0.00016586628,0.0002401189,0.008235249,0.00030710912,0.00043307303,0.019595083],"study_design_scores_gemma":[0.000002053208,0.000026969317,0.99719584,0.0000029293642,0.0000068632426,0.00007865727,0.000046267793,0.00033945948,0.001432881,0.00009996207,0.0007657349,0.0000022593495],"about_ca_topic_score_codex":0.0015444608,"about_ca_topic_score_gemma":0.0027995142,"teacher_disagreement_score":0.0019425665,"about_ca_system_score_codex":0.00014994688,"about_ca_system_score_gemma":0.00008259602,"threshold_uncertainty_score":0.003585875},"labels":[],"label_agreement":null},{"id":"W2900311665","doi":"10.3847/1538-4357/aaffd1","title":"Detection of the Temporal Variation of the Sun's Cosmic Ray Shadow with the IceCube Detector","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Snolab; University of Alberta","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Helmholtz Alliance for Astroparticle Physics; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Physics; Cosmic ray; Shadow (psychology); Astronomy; Astrophysics; COSMIC cancer database; Detector; Neutrino detector; Flux (metallurgy); Observatory; Neutrino; Neutrino oscillation; Optics; Nuclear physics","score_opus":0.004109904413325164,"score_gpt":0.18212310338212975,"score_spread":0.17801319896880458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2900311665","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989512,0.00029284175,0.0015419002,0.000034261247,0.000023058843,0.000014837277,0.0046427255,0.00008472311,0.0038536997],"genre_scores_gemma":[0.9902474,0.00012239566,0.0018262439,0.000026171463,0.000017284608,0.000018466999,0.0072122314,0.000023336328,0.00050638895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996643,0.000046190573,0.000020347095,0.00008642103,0.000120612174,0.00006213002],"domain_scores_gemma":[0.99845576,0.00023992009,0.00051656255,0.00021170915,0.00043663057,0.00013948658],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000763648,0.00021903298,0.00036081942,0.0011753343,0.00028059032,0.00059569394,0.00020542035,0.00018734831,0.0008197072],"category_scores_gemma":[0.0011035338,0.00012873615,0.0001568199,0.0014156522,0.0002690802,0.0003289958,0.00050280953,0.00029381088,0.00021360873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005667876,0.00008149767,0.9599441,0.00007312465,0.00013992566,0.00020883488,0.00020686655,0.0017082107,0.021014873,0.00030810595,0.0015658084,0.014181891],"study_design_scores_gemma":[0.0000062321205,0.00008255648,0.98627275,0.0000121754665,0.00003163936,0.00022323924,0.000074760814,0.0022289155,0.0070139454,0.00008501358,0.0039583333,0.000010387338],"about_ca_topic_score_codex":0.0063638813,"about_ca_topic_score_gemma":0.014447363,"teacher_disagreement_score":0.0063638813,"about_ca_system_score_codex":0.0004175585,"about_ca_system_score_gemma":0.0002864425,"threshold_uncertainty_score":0.012653649},"labels":[],"label_agreement":null},{"id":"W2900589768","doi":"10.3847/1538-4357/aaf38e","title":"Observational Signatures of Planets in Protoplanetary Disks: Planet-induced Line Broadening in Gaps","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Planet; Radiative transfer; Line (geometry); Protoplanet; Thermal; Accretion (finance); Kinematics; Gravitation; Opacity; Transonic","score_opus":0.019524463816504956,"score_gpt":0.2515232703979399,"score_spread":0.23199880658143496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2900589768","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99936646,0.000031385156,0.00027855168,0.000013406805,9.187165e-7,0.0000013186161,0.00003749461,0.00002226959,0.0002481202],"genre_scores_gemma":[0.99984455,0.0000054990705,0.000110256246,0.000002242198,7.393012e-7,6.8687626e-7,0.000016334248,0.0000030231895,0.000016707323],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996984,0.000005304256,0.0000012244325,0.000009491655,0.000006411898,0.000007694666],"domain_scores_gemma":[0.99979657,0.000048935974,0.00007492129,0.000025267724,0.00001252476,0.000041801668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001100692,0.000123722,0.0001122993,0.00021896572,0.00019861267,0.0002851466,0.00021601553,0.00029130644,0.00055255374],"category_scores_gemma":[0.00034844675,0.00011757787,0.00014836238,0.00015823843,0.00024443993,0.00032974192,0.0003399975,0.00020711901,0.00007683709],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089529715,0.00033271732,0.6236604,0.0001126547,0.00011692838,0.0010057384,0.0006487806,0.038128845,0.32143927,0.0018407817,0.000537466,0.011281199],"study_design_scores_gemma":[0.00007646446,0.00020990106,0.8478322,0.000014136005,0.000036826932,0.00044816444,0.00042913595,0.116662666,0.03202148,0.001347958,0.0009026412,0.000018409453],"about_ca_topic_score_codex":0.00066996,"about_ca_topic_score_gemma":0.0005139996,"teacher_disagreement_score":0.00066996,"about_ca_system_score_codex":0.00017970215,"about_ca_system_score_gemma":0.0000506969,"threshold_uncertainty_score":0.0018485188},"labels":[],"label_agreement":null},{"id":"W2900657062","doi":"10.3847/1538-4357/aaf23f","title":"On a New Method to Estimate the Distance, Reddening, and Metallicity of RR Lyrae Stars Using Optical/Near-infrared (B, V, I, J, H, K) Mean Magnitudes: ω Centauri as a First Test Case","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Distance modulus; RR Lyrae variable; Metallicity; Standard deviation; Absolute magnitude; Overtone; Homogeneous; Stars","score_opus":0.014199756102820935,"score_gpt":0.292332182494013,"score_spread":0.27813242639119207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2900657062","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.18016687,0.00032445422,0.813982,0.00010637993,0.000059311074,0.000068891604,0.0006733878,0.0020330576,0.00258565],"genre_scores_gemma":[0.5734703,0.000123959,0.42351624,0.00006128556,0.00006561169,0.00011345563,0.0007014754,0.0002663393,0.0016813435],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99934775,0.00016657468,0.000038045906,0.00021809155,0.00018768545,0.00004197493],"domain_scores_gemma":[0.9981704,0.00072910887,0.0002535142,0.00036214944,0.00039807954,0.000086791864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010711434,0.00064842857,0.00056430214,0.0032913412,0.00032213202,0.0010708944,0.0006836848,0.00042638462,0.0015471455],"category_scores_gemma":[0.0042856433,0.00039225095,0.0005772466,0.00091517414,0.00033593972,0.0005981218,0.0008899968,0.0006859158,0.00065136043],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036359375,0.0002414248,0.19397521,0.00021561312,0.00057947834,0.0003329048,0.0007029391,0.093259744,0.10435635,0.012770093,0.0031580038,0.5900447],"study_design_scores_gemma":[0.0000804691,0.00013669653,0.114364155,0.00004185525,0.00010262301,0.0005104064,0.00012830067,0.8443102,0.025030747,0.00674224,0.008389681,0.00016257097],"about_ca_topic_score_codex":0.002920423,"about_ca_topic_score_gemma":0.004178316,"teacher_disagreement_score":0.0032913412,"about_ca_system_score_codex":0.00041151352,"about_ca_system_score_gemma":0.0003142989,"threshold_uncertainty_score":0.005806923},"labels":[],"label_agreement":null},{"id":"W2900962508","doi":"10.3847/1538-4357/aaf057","title":"Spatially Resolved [C ii] Emission in SPT0346-52: A Hyper-starburst Galaxy Merger at z ∼ 5.7","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; National Astronomical Observatory of Japan; Flatiron Health; Gordon and Betty Moore Foundation; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Galaxy; Galaxy merger; Line (geometry); Star formation; Emission spectrum; Line-of-sight","score_opus":0.006583647037001332,"score_gpt":0.20539199406624128,"score_spread":0.19880834702923994,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2900962508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992111,0.000025093712,0.0001568203,0.000019198776,0.0000018930576,0.0000023972814,0.00016898653,0.000021516009,0.00039290788],"genre_scores_gemma":[0.99944586,0.000008444302,0.00024346904,0.000013452596,0.000003345545,0.0000014895232,0.00020658123,0.0000058028095,0.000071568844],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999242,0.0000065857735,0.00000436713,0.000024399373,0.000017887447,0.000022582308],"domain_scores_gemma":[0.99971086,0.000019747351,0.000092642935,0.000020756419,0.00003139513,0.00012470393],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011678419,0.00020135366,0.00027893102,0.00048414822,0.00044788248,0.0005388003,0.00039545758,0.00030587427,0.0011843927],"category_scores_gemma":[0.00021181164,0.00020038817,0.00022232096,0.00053089904,0.00026856374,0.0001903957,0.00042604477,0.00030369728,0.00031047696],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006245044,0.00027161159,0.75760704,0.000036160036,0.00010305113,0.0038724677,0.00066766347,0.0013441563,0.22629675,0.00030366852,0.0007932931,0.00807951],"study_design_scores_gemma":[0.000015003541,0.00007455568,0.9928041,0.0000036498054,0.000018407109,0.0010352158,0.00018520161,0.0023255977,0.0031344637,0.00006210522,0.00033597625,0.000005649157],"about_ca_topic_score_codex":0.00736699,"about_ca_topic_score_gemma":0.009792758,"teacher_disagreement_score":0.00736699,"about_ca_system_score_codex":0.00036364552,"about_ca_system_score_gemma":0.00013071968,"threshold_uncertainty_score":0.014648199},"labels":[],"label_agreement":null},{"id":"W2901092239","doi":"10.3847/1538-4357/ab0f3b","title":"Multi-epoch Direct Imaging and Time-variable Scattered Light Morphology of the HD 163296 Protoplanetary Disk","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Protoplanet; Protoplanetary disk; Subaru Telescope; Coronagraph; Exoplanet; Debris disk; Brightness; Planet; Surface brightness","score_opus":0.0046686193693266905,"score_gpt":0.20534209980336482,"score_spread":0.20067348043403813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901092239","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99701357,0.00012175909,0.00023751223,0.000026146648,0.0000065554405,0.0000063803463,0.0006381996,0.00004643862,0.0019034223],"genre_scores_gemma":[0.9978059,0.0000539306,0.0007364494,0.000023212278,0.000010048507,0.000004412705,0.0009454737,0.000012413967,0.00040826292],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995184,0.0000027235862,0.0000026466064,0.000016238735,0.000016592214,0.00001002471],"domain_scores_gemma":[0.99986136,0.000007946505,0.000033912896,0.000015338808,0.000022144852,0.00005915716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000094132156,0.00017557557,0.00014744244,0.0007213617,0.00028978018,0.0002456806,0.00020012124,0.00026687706,0.0010111203],"category_scores_gemma":[0.00013348681,0.0001336845,0.00019148352,0.00034100932,0.00013342102,0.00016223117,0.0003494046,0.00021313653,0.00030334914],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007181365,0.00020769713,0.33298293,0.00011158588,0.00010623156,0.0025195547,0.0005486942,0.0024536327,0.6384185,0.00027348023,0.0014893975,0.020170247],"study_design_scores_gemma":[0.000010978639,0.00006125694,0.9911686,0.0000059784675,0.000012302214,0.000737533,0.000093681345,0.0016010866,0.005445488,0.00004521303,0.00081078894,0.0000070124047],"about_ca_topic_score_codex":0.0022943388,"about_ca_topic_score_gemma":0.006286952,"teacher_disagreement_score":0.0022943388,"about_ca_system_score_codex":0.00022288764,"about_ca_system_score_gemma":0.00009883724,"threshold_uncertainty_score":0.0045620203},"labels":[],"label_agreement":null},{"id":"W2901098887","doi":"10.3847/1538-4357/aaf1b4","title":"An Enormous Molecular Gas Flow in the RX J0821+0752 Galaxy Cluster","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Cooling flow; Galaxy; Cluster (spacecraft); Galaxy cluster; Plume; Molecular cloud; Line (geometry); Active galactic nucleus","score_opus":0.004042348938465446,"score_gpt":0.20322415053876525,"score_spread":0.1991818016002998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901098887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988293,0.0000845929,0.00007246484,0.000039539034,0.0000034705156,0.000002730411,0.00015217256,0.00004466295,0.0007710202],"genre_scores_gemma":[0.99899155,0.000043384956,0.0002102818,0.000016129992,0.00001448761,0.0000036150973,0.00043795945,0.000007678457,0.00027482182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992263,0.000004355149,0.0000025795753,0.00002951112,0.000016012298,0.000024888897],"domain_scores_gemma":[0.999869,0.000010543525,0.000029058823,0.000017812412,0.000017698285,0.000055927743],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000079674675,0.00020144103,0.00021028132,0.000782265,0.00051535753,0.00060504087,0.0003029468,0.0002504665,0.0011776609],"category_scores_gemma":[0.00018233949,0.0001626103,0.00014616428,0.00043581915,0.00031112204,0.00027178487,0.000530163,0.00017858214,0.0002563029],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096863916,0.0002973241,0.61850923,0.00012824536,0.0002316658,0.003964645,0.0011868639,0.0061597885,0.3340649,0.0031828408,0.004085562,0.027220314],"study_design_scores_gemma":[0.00002443819,0.00008755559,0.98986685,0.000006825977,0.000038886887,0.00037589934,0.00019984799,0.002609205,0.0035234047,0.00017089552,0.0030788328,0.000017138016],"about_ca_topic_score_codex":0.009286192,"about_ca_topic_score_gemma":0.010667221,"teacher_disagreement_score":0.009286192,"about_ca_system_score_codex":0.00083773275,"about_ca_system_score_gemma":0.00023641945,"threshold_uncertainty_score":0.018464267},"labels":[],"label_agreement":null},{"id":"W2901577191","doi":"10.3847/1538-4357/aaee67","title":"Erratum: “The Sloan Digital Sky Survey Reverberation Mapping Project: Hα and Hβ Reverberation Measurements from First-year Spectroscopy and Photometry” (2017, ApJ, 851, 21)","year":2018,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; York University","funders":"","keywords":"Physics; Sky; Photometry (optics); Reverberation; Astronomy; Reverberation mapping; Astrophysics; Spectroscopy; Galaxy; Stars; Acoustics; Active galactic nucleus","score_opus":0.031910687160699405,"score_gpt":0.2516249607242806,"score_spread":0.2197142735635812,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901577191","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00050943444,0.000592511,0.0002593473,0.046700645,0.93791795,0.000026404672,0.0030873371,0.00042700046,0.010479327],"genre_scores_gemma":[0.014051167,0.004590339,0.0029482637,0.095524505,0.2627808,0.00017884687,0.013976266,0.0026657805,0.60328406],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.997598,0.00019314184,0.0004506758,0.0003142509,0.0012278196,0.00021613167],"domain_scores_gemma":[0.98637486,0.0017521732,0.0009258567,0.0008750951,0.009392188,0.0006798272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019123489,0.0018648258,0.0014016745,0.0037853029,0.0052669095,0.004209365,0.002265794,0.0048060953,0.054663282],"category_scores_gemma":[0.023636812,0.0007872525,0.0010506376,0.0022030943,0.0016572586,0.0032814606,0.0024466095,0.0073300437,0.048117604],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000016018517,0.000007771479,0.00007398741,0.000023984918,0.000002309223,0.00009013902,0.000012453885,0.00001778036,0.000033549637,0.00025855785,0.99759597,0.0018675377],"study_design_scores_gemma":[0.000019817704,0.000017068962,0.001591381,0.00016360167,0.000014065326,0.00014882542,0.00015478951,0.000113884984,0.00033253088,0.0008953823,0.9965203,0.00002838636],"about_ca_topic_score_codex":0.035516154,"about_ca_topic_score_gemma":0.041182786,"teacher_disagreement_score":0.054663282,"about_ca_system_score_codex":0.0043309713,"about_ca_system_score_gemma":0.0064007756,"threshold_uncertainty_score":0.18286693},"labels":[],"label_agreement":null},{"id":"W2901725520","doi":"10.3847/1538-4357/ab61f0","title":"The Density Structure of Simulated Stellar Streams","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"STREAMS; Environmental science; Computer science","score_opus":0.006049652299085269,"score_gpt":0.19805764588442856,"score_spread":0.1920079935853433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901725520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997396,0.0000150959095,0.0013692153,0.000037024667,0.000005820275,0.000009624559,0.00022375883,0.00009512934,0.00084839866],"genre_scores_gemma":[0.9978446,0.000008740063,0.0013148586,0.000012343003,0.0000022650624,0.00001559967,0.00051010615,0.000020120433,0.0002713232],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997676,0.00006873798,0.000014955142,0.00004537518,0.000050829083,0.0000526761],"domain_scores_gemma":[0.9983859,0.0008527011,0.00014464177,0.00015327403,0.00029282965,0.00017076921],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004901556,0.00029707458,0.00043334163,0.00052277587,0.0004806595,0.0007711742,0.0009497771,0.0006831113,0.0015214048],"category_scores_gemma":[0.0026727875,0.00031869303,0.00041869032,0.0005064462,0.0006548479,0.00037810046,0.00045431874,0.0004985934,0.00013912545],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001781525,0.000099095916,0.02180483,0.000015552636,0.0000452335,0.00012033577,0.000056215405,0.97298694,0.0015918906,0.0011872688,0.00030225416,0.0016122251],"study_design_scores_gemma":[0.0000299863,0.000033934208,0.0033798434,0.0000032368591,0.000008462341,0.000013240252,0.00002516443,0.99533916,0.00079489255,0.00026998483,0.00009600028,0.0000061515134],"about_ca_topic_score_codex":0.014903465,"about_ca_topic_score_gemma":0.007988346,"teacher_disagreement_score":0.014903465,"about_ca_system_score_codex":0.0010285352,"about_ca_system_score_gemma":0.0006333744,"threshold_uncertainty_score":0.029633403},"labels":[],"label_agreement":null},{"id":"W2901886793","doi":"10.3847/1538-4357/ab0e0c","title":"The Formation of Compact Elliptical Galaxies in the Vicinity of a Massive Galaxy: The Role of Ram-pressure Confinement","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; McMaster University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Elliptical galaxy; Ram pressure; Metallicity; Star formation; Supernova; Stars; Smoothed-particle hydrodynamics; Galaxy formation and evolution; Satellite galaxy","score_opus":0.005971248147082236,"score_gpt":0.21225274353812834,"score_spread":0.2062814953910461,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2901886793","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967385,0.00009862822,0.0008382031,0.00017317617,0.000008896506,0.000006940443,0.000058140668,0.000031832737,0.0020456503],"genre_scores_gemma":[0.99949265,0.00003009768,0.00029312572,0.000018889044,0.0000050001845,0.0000024482881,0.00002941466,0.0000066832245,0.000121591765],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990654,0.000034406414,0.0000041356047,0.000021257525,0.000010711486,0.000022943625],"domain_scores_gemma":[0.9995053,0.00012902523,0.000107773165,0.00005608833,0.000031441916,0.00017036109],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038739876,0.0003373094,0.00038305635,0.0002681339,0.0006434752,0.0015734626,0.0007906687,0.0007563078,0.0014420863],"category_scores_gemma":[0.0012799388,0.00023886647,0.00042021935,0.00016530878,0.0012941516,0.00084568124,0.00097302074,0.0004802798,0.00014442144],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005255074,0.0004202249,0.22970831,0.00015335345,0.00030924924,0.0010993767,0.000554063,0.71397924,0.021364877,0.02533621,0.0016144695,0.004935115],"study_design_scores_gemma":[0.00021236556,0.00021492028,0.08307859,0.000020239717,0.00007974773,0.00015238982,0.00028437714,0.9055446,0.0016084947,0.007973698,0.0007927257,0.00003787069],"about_ca_topic_score_codex":0.00922143,"about_ca_topic_score_gemma":0.0043761185,"teacher_disagreement_score":0.00922143,"about_ca_system_score_codex":0.00065598736,"about_ca_system_score_gemma":0.0003537622,"threshold_uncertainty_score":0.018335521},"labels":[],"label_agreement":null},{"id":"W2902022077","doi":"10.3847/1538-4357/aaf652","title":"Catalog of High Protostellar Surface Density Regions in Nearby Embedded Clusters","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Protostar; Star formation; RADIUS; Molecular cloud; Accretion (finance); Stars; Star cluster; Stellar evolution","score_opus":0.008414448926517696,"score_gpt":0.22638496814227296,"score_spread":0.21797051921575528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902022077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99848795,0.00016199746,0.00008757404,0.000005897725,8.4168136e-7,0.000004230143,0.0009179826,0.000018540033,0.0003149875],"genre_scores_gemma":[0.9954788,0.00010644328,0.00030447735,0.0000045429415,0.0000034337245,0.0000053752533,0.003781044,0.0000063059324,0.000309631],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997985,0.000017397217,0.00002017264,0.000054018357,0.000066491004,0.00004351273],"domain_scores_gemma":[0.99847585,0.00018627688,0.0005600997,0.00019843731,0.00020419217,0.00037507474],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025668024,0.00014846413,0.00022502661,0.004011905,0.00038561926,0.00049489044,0.00030884644,0.00015513835,0.0016210907],"category_scores_gemma":[0.0009813887,0.00010282132,0.00014591753,0.0031501139,0.00020115294,0.00023953653,0.00056604506,0.0000760863,0.00037527506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000058514503,0.000018058894,0.98932856,0.000034556797,0.000035706656,0.00011644282,0.00022803375,0.0002986143,0.0028896756,0.00012760588,0.0004197812,0.006444381],"study_design_scores_gemma":[0.0000033326642,0.000014648836,0.99806374,0.000006116049,0.000010951149,0.0001447829,0.00013965486,0.00031395594,0.00037169727,0.000039066992,0.000888986,0.0000029882185],"about_ca_topic_score_codex":0.0051196665,"about_ca_topic_score_gemma":0.008707111,"teacher_disagreement_score":0.0051196665,"about_ca_system_score_codex":0.00023490323,"about_ca_system_score_gemma":0.00025269552,"threshold_uncertainty_score":0.010179758},"labels":[],"label_agreement":null},{"id":"W2902028458","doi":"10.3847/1538-4357/aaf4fd","title":"The Next Generation Virgo Cluster Survey. XXIII. Fundamentals of Nuclear Star Clusters over Seven Decades in Galaxy Mass","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":144,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Stellar mass; Virgo Cluster; Star formation; Globular cluster; Galaxy cluster","score_opus":0.01615647440469366,"score_gpt":0.22906944874101692,"score_spread":0.21291297433632325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902028458","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94881845,0.005053275,0.0010086916,0.00046461204,0.000033370558,0.000033161556,0.03775422,0.00011519921,0.0067190174],"genre_scores_gemma":[0.97103304,0.0009112111,0.0011186682,0.000062340616,0.00002786761,0.000029364195,0.025416667,0.000026693142,0.0013739916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998167,0.000024935438,0.000011997483,0.000065740125,0.000042729724,0.000037865393],"domain_scores_gemma":[0.9993691,0.00008307545,0.00024344641,0.000079646474,0.00011149861,0.00011327811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004327121,0.00019060823,0.00016244696,0.0026052783,0.00021941737,0.000533888,0.0002836983,0.00021135429,0.0009798014],"category_scores_gemma":[0.0010843374,0.000113357535,0.00024929526,0.0025535307,0.000220517,0.00040404272,0.000730933,0.00019590787,0.000457237],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004565515,0.000010606411,0.9706487,0.00007749726,0.0000986361,0.000050647046,0.00027577885,0.00074464764,0.0016712938,0.0008419913,0.0041986136,0.02133586],"study_design_scores_gemma":[6.169783e-7,0.000004293883,0.9961151,0.0000072840667,0.0000061151727,0.000030569918,0.00004671774,0.00026832926,0.00011235566,0.00008235636,0.0033241548,0.0000021559542],"about_ca_topic_score_codex":0.026780732,"about_ca_topic_score_gemma":0.029712629,"teacher_disagreement_score":0.026780732,"about_ca_system_score_codex":0.0005712852,"about_ca_system_score_gemma":0.00022916342,"threshold_uncertainty_score":0.053249657},"labels":[],"label_agreement":null},{"id":"W2902454806","doi":"10.3847/1538-4357/aaf3b1","title":"The JCMT Transient Survey: An Extraordinary Submillimeter Flare in the T Tauri Binary System JW 566","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Canadian Space Agency; Korea Astronomy and Space Science Institute; Chinese Academy of Sciences; Academia Sinica","keywords":"Flare; Luminosity; Brightness; T Tauri star; Solar flare; Spectral index; Flux (metallurgy); Flare star; Binary system","score_opus":0.013441989164887933,"score_gpt":0.23742016828846593,"score_spread":0.223978179123578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902454806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989784,0.000027769525,0.000031048323,0.000015589507,0.0000032125577,0.0000062378645,0.0003998049,0.0000070989404,0.00053083804],"genre_scores_gemma":[0.99866605,0.000034155866,0.000082658655,0.00001495791,0.000011118754,0.000004515646,0.0008445938,0.0000042398206,0.00033779937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987006,0.000006673918,0.0000130922435,0.000029063567,0.000038889604,0.00004223045],"domain_scores_gemma":[0.9995208,0.000019799314,0.00021280728,0.00003352799,0.000044160024,0.0001688562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001513141,0.00015848607,0.00023339718,0.0009697972,0.0006118527,0.00046294014,0.00023134648,0.0002634339,0.0011639284],"category_scores_gemma":[0.00038954295,0.000106208565,0.00016963706,0.0008217949,0.0001998638,0.0002653016,0.0008031597,0.00023731602,0.0003478286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003215522,0.00010663173,0.9668959,0.000030231284,0.000038959635,0.0012734239,0.00042850553,0.00012190251,0.023016185,0.00008768761,0.00066005794,0.00701888],"study_design_scores_gemma":[0.000004498394,0.00003757726,0.9981006,0.0000026779467,0.0000065302293,0.0004777846,0.00010013448,0.00010492813,0.00048761594,0.000009482373,0.00066612056,0.0000020847656],"about_ca_topic_score_codex":0.009354352,"about_ca_topic_score_gemma":0.014422699,"teacher_disagreement_score":0.009354352,"about_ca_system_score_codex":0.0003924673,"about_ca_system_score_gemma":0.00019436154,"threshold_uncertainty_score":0.018599808},"labels":[],"label_agreement":null},{"id":"W2902986756","doi":"10.3847/1538-4357/ab1f10","title":"Cluster Cosmology Constraints from the 2500 deg<sup>2</sup> SPT-SZ Survey: Inclusion of Weak Gravitational Lensing Data from Magellan and the Hubble Space Telescope","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":367,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Université de Montréal; McGill University; Canadian Institute for Advanced Research","funders":"SLAC National Accelerator Laboratory; Ames Research Center; Bundesministerium für Wirtschaft und Technologie; Universities Space Research Association; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Argonne National Laboratory; U.S. Department of Energy; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; University of Chicago; National Science Foundation","keywords":"Weak gravitational lensing; Galaxy cluster; Cosmology; Dark energy; Redshift; Halo; Observable; Hubble's law; Galaxy; Gravitational lens","score_opus":0.014405250264590634,"score_gpt":0.23146765199992173,"score_spread":0.2170624017353311,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2902986756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963456,0.000043147207,0.0006351254,0.000050584527,0.000002180458,0.000006472405,0.0018493376,0.000020942893,0.0010466808],"genre_scores_gemma":[0.99568164,0.000026518948,0.00061708497,0.00001704907,0.000006952571,0.0000047459057,0.00352319,0.0000094584175,0.000113269445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994677,0.00014916086,0.000043282245,0.00009310519,0.00014438083,0.00010236484],"domain_scores_gemma":[0.99560165,0.0015555316,0.0010773235,0.0006022453,0.00047559993,0.00068769004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001292831,0.00046424224,0.00057431,0.001249941,0.0004601052,0.0012493767,0.0006116492,0.00027736404,0.0027259209],"category_scores_gemma":[0.006757351,0.00022257611,0.0004678805,0.0014556042,0.00037550213,0.00033712553,0.0007462647,0.00026124512,0.0006370094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023151604,0.000017070408,0.9831592,0.000024103687,0.00011848116,0.0001311203,0.00007973946,0.0073952987,0.0033212884,0.0007007693,0.00095849053,0.0038629288],"study_design_scores_gemma":[0.000017770928,0.00003006867,0.98518085,0.000007330585,0.000065986475,0.00007460614,0.00010519206,0.012208918,0.0011048313,0.0002814812,0.0009133752,0.00000953657],"about_ca_topic_score_codex":0.027085418,"about_ca_topic_score_gemma":0.02866494,"teacher_disagreement_score":0.027085418,"about_ca_system_score_codex":0.00046411416,"about_ca_system_score_gemma":0.0006466151,"threshold_uncertainty_score":0.05385554},"labels":[],"label_agreement":null},{"id":"W2903740919","doi":"10.3847/1538-4357/aaf7a4","title":"Multiband Optical and Near-Infrared Properties of Faint Submillimeter Galaxies with Serendipitous ALMA Detections","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Galaxy; Astrophysics; Redshift; Photometry (optics); Astronomy; Photometric redshift; Luminous infrared galaxy; Chandra Deep Field South; Submillimeter Array; Star formation; Stars","score_opus":0.00661859113111785,"score_gpt":0.18234387834412125,"score_spread":0.1757252872130034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2903740919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990344,0.00008067073,0.000054195985,0.0000071304084,0.0000016454945,0.0000023246012,0.00042987478,0.000011839349,0.0003779276],"genre_scores_gemma":[0.99885225,0.000044405744,0.000086350665,0.000007996224,0.0000066411003,0.0000030178946,0.0007897962,0.0000028503612,0.00020668215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981993,0.000021973054,0.000020812322,0.000045878223,0.000042686563,0.00004871329],"domain_scores_gemma":[0.998362,0.0002293889,0.0008057874,0.00016517066,0.00015522235,0.00028239278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029305305,0.00023883596,0.00022543676,0.002569493,0.00025660978,0.0005804847,0.00025504507,0.00017335842,0.0022382117],"category_scores_gemma":[0.0012277242,0.00011905151,0.00022255722,0.00097612006,0.0002052056,0.00032409458,0.0004582314,0.0001349117,0.0005807738],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003257169,0.00001721348,0.9962435,0.0000038367393,0.000015683205,0.000033378532,0.000054982844,0.000052692747,0.0013004936,0.00002621453,0.00012656015,0.002092839],"study_design_scores_gemma":[0.0000013035632,0.00001808927,0.9993748,0.0000019943423,0.0000068099803,0.00008765583,0.000044551638,0.000099186596,0.00020638696,0.000011474917,0.00014672535,9.963321e-7],"about_ca_topic_score_codex":0.0023884154,"about_ca_topic_score_gemma":0.003550786,"teacher_disagreement_score":0.002569493,"about_ca_system_score_codex":0.0001490751,"about_ca_system_score_gemma":0.000079759215,"threshold_uncertainty_score":0.007487595},"labels":[],"label_agreement":null},{"id":"W2903742437","doi":"10.3847/1538-4357/aaf860","title":"The ISM Properties and Gas Kinematics of a Redshift 3 Massive Dusty Star-forming Galaxy","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; University of California, Los Angeles; Max-Planck-Gesellschaft; Smithsonian Institution; National Science Council; Rutgers, The State University of New Jersey; Flatiron Health; National Radio Astronomy Observatory; Space Telescope Science Institute; Gordon and Betty Moore Foundation; National Science Foundation; James S. McDonnell Foundation; Academia Sinica; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Plateau de Bure Interferometer; Galaxy; Redshift; Star formation; Emission spectrum; Submillimeter Array; Line (geometry); Galaxy rotation curve; Interstellar medium","score_opus":0.013000840755441173,"score_gpt":0.2177730115124167,"score_spread":0.20477217075697554,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2903742437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99979156,0.000020566835,0.000034236615,0.000004175741,2.7261103e-7,9.4463815e-7,0.000032429885,0.0000032679543,0.000112579284],"genre_scores_gemma":[0.99977046,0.000009759034,0.00007481545,0.000005551999,0.0000013249237,4.676409e-7,0.000080350736,5.2892153e-7,0.000056720706],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995255,0.0000060211346,0.0000031173931,0.0000123674145,0.0000099529,0.000016024112],"domain_scores_gemma":[0.9999032,0.000010289251,0.000024301025,0.0000072939724,0.0000063134726,0.000048515012],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009034989,0.0001541,0.00012952568,0.00042321553,0.00020090528,0.00030453113,0.00013311212,0.000116273484,0.0008320168],"category_scores_gemma":[0.00013666353,0.00007977914,0.00010931849,0.00022407684,0.0001762922,0.000113852606,0.00020792474,0.00008458497,0.00014633972],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010265213,0.00006365609,0.97345406,0.000006971143,0.000024770445,0.00028674884,0.00032952553,0.0002618086,0.021880537,0.00016588692,0.000118411204,0.0033048764],"study_design_scores_gemma":[0.0000037246436,0.00005452313,0.998432,0.0000011052791,0.0000054701586,0.00016355714,0.000099806144,0.00040254032,0.0006383808,0.000026707025,0.00017114329,9.896695e-7],"about_ca_topic_score_codex":0.004584597,"about_ca_topic_score_gemma":0.0035770258,"teacher_disagreement_score":0.004584597,"about_ca_system_score_codex":0.00020194604,"about_ca_system_score_gemma":0.000051343217,"threshold_uncertainty_score":0.009115875},"labels":[],"label_agreement":null},{"id":"W2903857420","doi":"10.3847/1538-4357/aae9e6","title":"Spectroscopy of the K0 Binary Giant α UMa","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Radial velocity; Line (geometry); Absolute magnitude; Spectral line; Giant star; Stars; Astronomy; Geometry","score_opus":0.009711559456829725,"score_gpt":0.23378438492013132,"score_spread":0.2240728254633016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2903857420","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987348,0.00015644448,0.00015851126,0.000017336015,0.000004338309,0.0000041235676,0.00012690347,0.000013491895,0.0007840683],"genre_scores_gemma":[0.9988531,0.00006558532,0.00026201725,0.000023095645,0.0000051569928,0.0000026747007,0.0003182341,0.0000036628378,0.0004665337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999261,0.0000050747744,0.0000044721646,0.000024292916,0.000016487791,0.000023585597],"domain_scores_gemma":[0.9997962,0.000012924034,0.00007768107,0.000015229149,0.000033846845,0.0000640591],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001707425,0.00020096201,0.00017602732,0.00070879614,0.00058919785,0.00035316663,0.00018860852,0.00029809002,0.0007226036],"category_scores_gemma":[0.0002023863,0.00012573374,0.00012219661,0.00049166917,0.00016655159,0.00023634349,0.00027535445,0.00019595887,0.0002358741],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043905753,0.00010976778,0.49652064,0.00010964517,0.00007095885,0.0011548639,0.00078272447,0.00045367866,0.48609927,0.00020154641,0.000721376,0.0133363865],"study_design_scores_gemma":[0.000008562776,0.00016768885,0.9831933,0.000014602757,0.000021964339,0.0006909198,0.00025636153,0.0006089809,0.012836347,0.000049954404,0.002144094,0.000007408445],"about_ca_topic_score_codex":0.0026009947,"about_ca_topic_score_gemma":0.0042048027,"teacher_disagreement_score":0.0026009947,"about_ca_system_score_codex":0.0004747178,"about_ca_system_score_gemma":0.00011641716,"threshold_uncertainty_score":0.0051716566},"labels":[],"label_agreement":null},{"id":"W2904353158","doi":"10.3847/1538-4357/ab1a3e","title":"The Time-domain Spectroscopic Survey: Radial Velocity Variability in Dwarf Carbon Stars","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Stars; Carbon star; Radial velocity; White dwarf; Binary star; Binary number; Asymptotic giant branch; Binary system; Mass distribution","score_opus":0.006892205732134674,"score_gpt":0.21510358769756893,"score_spread":0.20821138196543426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2904353158","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992286,0.000019085763,0.00025299808,0.0000060070506,5.0953935e-7,0.0000013894427,0.00029838734,0.000009296444,0.00018375696],"genre_scores_gemma":[0.99934024,0.000008713701,0.00017456445,0.0000021482076,0.0000012627601,0.00000121762,0.0004129366,0.000001811085,0.000056987832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998779,0.000024717761,0.000008758917,0.00003829158,0.000030555624,0.000019890545],"domain_scores_gemma":[0.99916184,0.00018404948,0.00031356578,0.00007968123,0.00014431035,0.00011643512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031184722,0.000103190345,0.00012353656,0.0012061313,0.00013919937,0.00022998184,0.00015172572,0.0001584699,0.00045758256],"category_scores_gemma":[0.0010321229,0.000057167254,0.00014798176,0.00080416905,0.00010596902,0.00012875051,0.0001869028,0.00009355362,0.00016491221],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006576593,0.00002520764,0.98792213,0.000006663746,0.000026585096,0.000031638487,0.000061057464,0.001225643,0.0058162543,0.000086558735,0.0001338716,0.004598643],"study_design_scores_gemma":[0.0000016210149,0.000019471974,0.99498343,0.0000012572405,0.000004211086,0.00008122257,0.000034855984,0.0039829365,0.0006558396,0.000034178815,0.00019858325,0.0000024583153],"about_ca_topic_score_codex":0.003942694,"about_ca_topic_score_gemma":0.0045834854,"teacher_disagreement_score":0.003942694,"about_ca_system_score_codex":0.00019420333,"about_ca_system_score_gemma":0.00009749751,"threshold_uncertainty_score":0.007839501},"labels":[],"label_agreement":null},{"id":"W2904387936","doi":"10.3847/1538-4357/aaf5cc","title":"All-sky Measurement of the Anisotropy of Cosmic Rays at 10 TeV and Mapping of the Local Interstellar Magnetic Field","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Snolab; University of Alberta","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Los Alamos National Laboratory; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Chiba University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Coordinación de la Investigación Científica; Villum Fonden; National Research Foundation of Korea; Consejo Nacional de Ciencia y Tecnología; Fonds Wetenschappelijk Onderzoek; Benemérita Universidad Autónoma de Puebla; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Laboratory Directed Research and Development; National Science Foundation; Belgian Federal Science Policy Office; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Cosmic ray; Heliosphere; Anisotropy; Interstellar medium; Sky; Magnetic field; Cherenkov radiation","score_opus":0.009585215934757939,"score_gpt":0.19344739982674206,"score_spread":0.1838621838919841,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2904387936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99015886,0.0001304004,0.0019981908,0.000032187832,0.000005860364,0.000007252855,0.0023235201,0.000081187194,0.005262544],"genre_scores_gemma":[0.99669397,0.00005669179,0.0014696763,0.000012048057,0.000006189896,0.0000035502114,0.0014674193,0.000014338797,0.00027612818],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999887,0.000025229985,0.0000048667866,0.000029706027,0.00003114501,0.000022102335],"domain_scores_gemma":[0.99965525,0.000051091967,0.00008743853,0.000059690305,0.00006802151,0.00007848747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023329373,0.0001841182,0.00015051315,0.00065200665,0.0001649045,0.00033308152,0.00015339395,0.00009720444,0.0014422938],"category_scores_gemma":[0.00039511692,0.00013279427,0.00013756986,0.0005610013,0.00016818433,0.00021498447,0.00031217473,0.00022030453,0.00038867904],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040082543,0.00005364701,0.80635315,0.00004985614,0.00017015492,0.00020433316,0.00014047805,0.00198463,0.17330459,0.00081583817,0.0008931386,0.015629534],"study_design_scores_gemma":[0.0000072103567,0.00002874521,0.98903465,0.000004032031,0.00001634281,0.00010357374,0.000040837458,0.001234729,0.0083426675,0.00012981497,0.0010517681,0.000005627665],"about_ca_topic_score_codex":0.0033263795,"about_ca_topic_score_gemma":0.014201722,"teacher_disagreement_score":0.0033263795,"about_ca_system_score_codex":0.00020900441,"about_ca_system_score_gemma":0.00015968611,"threshold_uncertainty_score":0.0066140294},"labels":[],"label_agreement":null},{"id":"W2904404514","doi":"10.3847/1538-4357/aaf4bf","title":"Erratum: “Virgo Redux: The Masses and Stellar Content of Nuclei in Early-type Galaxies from Multiband Photometry and Spectroscopy” (2017, ApJ, 849, 55)","year":2018,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Photometry (optics); Astrophysics; Galaxy; Astronomy; Spectroscopy; Stars","score_opus":0.023659836883104347,"score_gpt":0.2744938193257289,"score_spread":0.25083398244262456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2904404514","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0010572431,0.0009775445,0.00040196584,0.059490867,0.92418617,0.000020063237,0.0038649393,0.00065602787,0.00934513],"genre_scores_gemma":[0.02259317,0.0052337707,0.0037515895,0.10774926,0.29642534,0.000119922806,0.013107758,0.0028837577,0.54813534],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99869955,0.00011902054,0.0002221623,0.00022049103,0.0006286473,0.000110160334],"domain_scores_gemma":[0.9941148,0.0012237839,0.0005955849,0.00049172953,0.0031076248,0.00046644852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012709027,0.001593237,0.0011736198,0.0029543499,0.0031590236,0.0026834232,0.0017873563,0.0034319498,0.044739757],"category_scores_gemma":[0.016445044,0.00067831075,0.00087058934,0.0016139331,0.0013355267,0.0022207967,0.0018398463,0.0058165505,0.034114707],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000025122974,0.000008658066,0.0001802756,0.00003182002,0.0000043865266,0.0001072144,0.000014818456,0.000025853435,0.00006458235,0.0003362149,0.99623007,0.0029709416],"study_design_scores_gemma":[0.000026079622,0.000028028222,0.0034493099,0.00017907356,0.000023251441,0.00038525858,0.00013749952,0.00020799876,0.0005797403,0.0014959266,0.9934454,0.000042381937],"about_ca_topic_score_codex":0.019385355,"about_ca_topic_score_gemma":0.022907246,"teacher_disagreement_score":0.044739757,"about_ca_system_score_codex":0.002687083,"about_ca_system_score_gemma":0.0028839193,"threshold_uncertainty_score":0.14966941},"labels":[],"label_agreement":null},{"id":"W2904431202","doi":"10.3847/1538-4357/aae0ef","title":"QED Phenomena in an Ultrastrong Magnetic Field. I. Electron–Photon Scattering, Pair Creation, and Annihilation","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Photon; Pair production; Electron; Bremsstrahlung; Positron; Annihilation; Scattering; Magnetic field; Positronium; Atomic physics; Landau quantization; Context (archaeology); Quantum electrodynamics; Nuclear physics; Quantum mechanics","score_opus":0.007813862326126436,"score_gpt":0.3029512841105237,"score_spread":0.2951374217843973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2904431202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88245624,0.0018000498,0.06794101,0.00079670135,0.00016967759,0.000065138825,0.000120606055,0.00019685178,0.046453677],"genre_scores_gemma":[0.9938292,0.00026979388,0.002831346,0.000049617458,0.000040589926,0.000015356676,0.000021230708,0.000017564422,0.002925259],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99982846,0.000071882634,0.000005172416,0.000011557517,0.00004032085,0.00004270684],"domain_scores_gemma":[0.999323,0.0003629454,0.00013472055,0.00006757308,0.000063908614,0.000047874924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006180403,0.00041274837,0.0005030221,0.0007302552,0.00055717066,0.0007351604,0.0004948145,0.00043002222,0.002750357],"category_scores_gemma":[0.0016095325,0.00014975869,0.0003898058,0.0005699383,0.0014575912,0.00092458597,0.0007539475,0.00044108072,0.00018707271],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002811006,0.00011329915,0.0029423826,0.00020740443,0.000047288795,0.0006622703,0.0002290859,0.20694155,0.024726247,0.75595117,0.0007180962,0.0071800794],"study_design_scores_gemma":[0.00009610659,0.00012366271,0.002734624,0.000020376143,0.000023465705,0.000248362,0.00008859606,0.8531488,0.0066063865,0.13487266,0.0020045056,0.000032367174],"about_ca_topic_score_codex":0.0014155147,"about_ca_topic_score_gemma":0.00058170257,"teacher_disagreement_score":0.002750357,"about_ca_system_score_codex":0.0010493266,"about_ca_system_score_gemma":0.000264801,"threshold_uncertainty_score":0.009200871},"labels":[],"label_agreement":null},{"id":"W2904920060","doi":"10.3847/1538-4357/aaf71f","title":"Simultaneous X-Ray and Infrared Observations of Sagittarius A*'s Variability","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Flare; Sagittarius A*; Infrared; Galactic Center; Accretion (finance); Flux (metallurgy); Light curve","score_opus":0.010510987504990183,"score_gpt":0.2182590294866674,"score_spread":0.2077480419816772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2904920060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99781173,0.00005903139,0.0002748695,0.000018410718,0.000005080568,0.0000066087027,0.00091393385,0.00006719887,0.00084316265],"genre_scores_gemma":[0.9951894,0.000045650067,0.00085425,0.000021111187,0.00002197776,0.0000087942435,0.0036539324,0.000015528218,0.0001893336],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980694,0.000018175338,0.000013846031,0.0000644746,0.000055989483,0.000040573446],"domain_scores_gemma":[0.9993813,0.00005242521,0.00016829603,0.00007983955,0.0000983208,0.00021982873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034638977,0.00029803545,0.00034822992,0.0013914143,0.0004066857,0.0006737184,0.00026126628,0.0002465535,0.000628776],"category_scores_gemma":[0.00033737678,0.00019402917,0.00039818592,0.0007633988,0.00017076089,0.000273051,0.00075622275,0.0002828376,0.0002962069],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045635283,0.00024037066,0.87253237,0.000047088888,0.0004111163,0.00031911183,0.00033523806,0.0014826746,0.10270219,0.0001562145,0.0010084177,0.020308943],"study_design_scores_gemma":[0.000008395786,0.00007708959,0.9968177,0.000002736845,0.000025242509,0.000091987764,0.000057398425,0.0008975722,0.0012401035,0.00003075066,0.0007444961,0.000006541196],"about_ca_topic_score_codex":0.005555776,"about_ca_topic_score_gemma":0.009700727,"teacher_disagreement_score":0.005555776,"about_ca_system_score_codex":0.00024475987,"about_ca_system_score_gemma":0.00020686461,"threshold_uncertainty_score":0.011046886},"labels":[],"label_agreement":null},{"id":"W2905295886","doi":"10.3847/1538-4357/ab2638","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion Disk Sizes from Continuum Lags","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Reverberation mapping; Sky; Accretion disc; Monte Carlo method; Accretion (finance); Quasar; Markov chain Monte Carlo; Lag","score_opus":0.009077531782484455,"score_gpt":0.21096790975841248,"score_spread":0.20189037797592801,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2905295886","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9600129,0.00021411455,0.004933303,0.00010223689,0.000012548546,0.00002938887,0.029238833,0.00096151535,0.004495065],"genre_scores_gemma":[0.9504441,0.000113791764,0.0078030033,0.000037967046,0.000020674655,0.000054663113,0.040719397,0.0002369476,0.0005695807],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993443,0.00016480059,0.00004356162,0.00014560643,0.0002285125,0.000073233394],"domain_scores_gemma":[0.9967924,0.00057810545,0.0011166498,0.0005464532,0.0006438835,0.00032254698],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014531265,0.0004836969,0.00022362778,0.002568443,0.00025319232,0.0009771023,0.00040152812,0.00021216413,0.0012931568],"category_scores_gemma":[0.0035548392,0.00018861446,0.00026932862,0.001966406,0.000186604,0.00047861168,0.00068872387,0.0002628674,0.0010133813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017270636,0.00006559535,0.95267355,0.00007040763,0.00013144585,0.00008546536,0.00029752043,0.0041664867,0.0026769345,0.00042485297,0.010439887,0.028795097],"study_design_scores_gemma":[0.0000147891315,0.000016927337,0.9876386,0.000011373628,0.0000138763,0.00004894987,0.00006536537,0.0068050963,0.0019096989,0.00016751995,0.0032975469,0.000010274628],"about_ca_topic_score_codex":0.013074636,"about_ca_topic_score_gemma":0.014285042,"teacher_disagreement_score":0.013074636,"about_ca_system_score_codex":0.00035419347,"about_ca_system_score_gemma":0.00037351224,"threshold_uncertainty_score":0.025997043},"labels":[],"label_agreement":null},{"id":"W2905312720","doi":"10.3847/1538-4357/aaf886","title":"Constraining the Magnetic Field of the Smith High-velocity Cloud Using Faraday Rotation","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Dominion Astrophysical Observatory; University of British Columbia","funders":"","keywords":"Magnetic field; Faraday effect; Milky Way; Measure (data warehouse); Field (mathematics); Rotation (mathematics); L-shell; Magnetic cloud","score_opus":0.010028415761288254,"score_gpt":0.2342454537682957,"score_spread":0.22421703800700743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2905312720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940923,0.0001185931,0.0027140912,0.00003306028,0.0000052090422,0.0000099396075,0.00045543464,0.00005105098,0.0025203833],"genre_scores_gemma":[0.99857616,0.000028997927,0.0010544348,0.0000048566717,0.000003913884,0.0000018297686,0.00023123894,0.000003657212,0.000094955496],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988675,0.000014802337,0.0000037085902,0.000034737015,0.000030589013,0.000029348514],"domain_scores_gemma":[0.99957293,0.00010673122,0.00014528725,0.000048792186,0.00004120136,0.00008510036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002369493,0.0002879526,0.00029208543,0.0010160994,0.00046340263,0.0007549069,0.00031977287,0.0002624722,0.0010721863],"category_scores_gemma":[0.0008633388,0.00022140435,0.00023491352,0.0006635942,0.0002655081,0.00030454417,0.00039617656,0.00020423741,0.00025677547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001943937,0.000062168474,0.85847586,0.000046658315,0.00014011617,0.00029878196,0.00010822786,0.050750207,0.06997746,0.0017645959,0.0007356067,0.017445939],"study_design_scores_gemma":[0.00005673648,0.00008088728,0.8873926,0.00002259733,0.00003902667,0.00011126234,0.00010746873,0.0993362,0.009967887,0.00093999575,0.0019121711,0.000033144068],"about_ca_topic_score_codex":0.03510998,"about_ca_topic_score_gemma":0.05676093,"teacher_disagreement_score":0.03510998,"about_ca_system_score_codex":0.0007336851,"about_ca_system_score_gemma":0.0005094237,"threshold_uncertainty_score":0.069811225},"labels":[],"label_agreement":null},{"id":"W2905381653","doi":"10.3847/1538-4357/aaf85f","title":"The Galactic Magneto-ionic Medium Survey: Moments of the Faraday Spectra","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Toronto; National Research Council Canada; Canadian Institute for Theoretical Astrophysics; Okanagan College; Dominion Astrophysical Observatory","funders":"","keywords":"Faraday effect; Sky; Spectral line; Line-of-sight; Telescope; Pulsar; Faraday cage; Observatory","score_opus":0.005645978189240686,"score_gpt":0.21404485543154295,"score_spread":0.20839887724230227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2905381653","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929595,0.00018825686,0.00027121583,0.00003100117,0.000003987782,0.0000043041655,0.004656508,0.000040924588,0.0018443089],"genre_scores_gemma":[0.9932515,0.00011383795,0.00044386816,0.0000088574725,0.000012418964,0.000005364439,0.005712916,0.000014197489,0.00043706686],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998646,0.000025142257,0.000009285564,0.000042237956,0.00003211554,0.000026668578],"domain_scores_gemma":[0.99965024,0.00004297994,0.00012707627,0.000035050078,0.00006450909,0.000080175356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020399745,0.00019015225,0.0001880099,0.00212578,0.0001226678,0.00047664763,0.0001347781,0.00011354286,0.0010388577],"category_scores_gemma":[0.00046280754,0.00007953561,0.00017606861,0.0013920923,0.00009853855,0.00023396936,0.00043960378,0.00010958651,0.00042663308],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008812752,0.000008411308,0.98457587,0.000021983125,0.00006360913,0.000062780106,0.00013574671,0.00040918763,0.005103573,0.00010706564,0.00091627194,0.008507294],"study_design_scores_gemma":[0.0000019410872,0.000006389588,0.99853766,0.0000020296145,0.0000039323613,0.000042197957,0.00007040331,0.00015468705,0.00026478563,0.000018674886,0.00089519715,0.000002185397],"about_ca_topic_score_codex":0.0052961744,"about_ca_topic_score_gemma":0.009649893,"teacher_disagreement_score":0.0052961744,"about_ca_system_score_codex":0.00021266154,"about_ca_system_score_gemma":0.000097178214,"threshold_uncertainty_score":0.01053071},"labels":[],"label_agreement":null},{"id":"W2906720395","doi":"10.3847/1538-4357/aaf9a7","title":"Near-infrared Survey and Photometric Redshifts in the Extended GOODS-North Field","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Redshift; Photometry (optics); Photometric redshift; Hubble Deep Field; Limiting; Limiting magnitude; Outlier","score_opus":0.01535188550768761,"score_gpt":0.2435288618941027,"score_spread":0.2281769763864151,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2906720395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99546415,0.00013582186,0.0008287819,0.000018427478,0.0000049211294,0.0000071251065,0.002285237,0.000048557344,0.0012070718],"genre_scores_gemma":[0.9858155,0.00009767938,0.0016532515,0.000021781254,0.000012932365,0.000009355375,0.011383901,0.00001916825,0.0009864102],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967873,0.000051856605,0.000017194261,0.00010709603,0.00009072434,0.00005444532],"domain_scores_gemma":[0.9991567,0.00010124142,0.0002259981,0.00020673784,0.00017858019,0.00013081226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076273206,0.00021420205,0.00022700267,0.0017340761,0.00018587612,0.00042219405,0.00023607076,0.0001411531,0.0011418349],"category_scores_gemma":[0.000813679,0.000130172,0.00020617875,0.0013349017,0.00020699385,0.00027066565,0.000476512,0.0001346472,0.0005395017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010577768,0.00006357477,0.9765203,0.000033850938,0.00006653676,0.000100394056,0.00019981895,0.0018417026,0.0046464107,0.0003673742,0.0016222973,0.014431916],"study_design_scores_gemma":[0.000004332518,0.000008087929,0.99780697,0.0000032943437,0.00000872804,0.000022219236,0.000044005923,0.0006857662,0.00025243056,0.0000372,0.0011242854,0.0000026980197],"about_ca_topic_score_codex":0.01718691,"about_ca_topic_score_gemma":0.03078341,"teacher_disagreement_score":0.01718691,"about_ca_system_score_codex":0.00035690938,"about_ca_system_score_gemma":0.00021622756,"threshold_uncertainty_score":0.034173727},"labels":[],"label_agreement":null},{"id":"W2907506244","doi":"10.3847/1538-4357/ab1d49","title":"The Extended Baryon Oscillation Spectroscopic Survey: Measuring the Cross-correlation between the Mg ii Flux Transmission Field and Quasars and Galaxies at z = 0.59","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Agence Nationale de la Recherche; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Quasar; Redshift; Baryon; Galaxy; Flux (metallurgy); Baryon acoustic oscillations; Spectral line; Oscillation (cell signaling); Astronomy; Chemistry","score_opus":0.009909727560502183,"score_gpt":0.23094251447892433,"score_spread":0.22103278691842215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2907506244","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991466,0.00001962382,0.00013653404,0.000006774551,8.1514276e-7,0.000001310453,0.00028288056,0.000006051769,0.00039954402],"genre_scores_gemma":[0.9991755,0.000019247222,0.00016892832,0.000006129411,0.0000041233816,0.0000016519223,0.0004916432,0.0000021386393,0.00013049111],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984026,0.000035393074,0.0000105195995,0.000038346123,0.000046187648,0.000029207209],"domain_scores_gemma":[0.9987888,0.00020990895,0.000510761,0.00010796905,0.00015743238,0.00022515604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057536614,0.00012551177,0.00014902835,0.0011688147,0.00016192642,0.00029880306,0.00014696197,0.00010692039,0.0009835351],"category_scores_gemma":[0.0013138021,0.00011617873,0.0000862171,0.00070217875,0.00016240127,0.00023386854,0.0004662963,0.00016029067,0.00024591378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036552778,0.000009990887,0.99551326,0.000003150483,0.000017516266,0.0000100991165,0.000060834995,0.000048024493,0.0021529554,0.000043173906,0.00006851548,0.0020359291],"study_design_scores_gemma":[0.0000010614671,0.000008280416,0.9995604,7.263811e-7,0.0000032466182,0.000012464814,0.000024936036,0.000111131696,0.00018447284,0.0000073276306,0.00008528339,7.127169e-7],"about_ca_topic_score_codex":0.005971504,"about_ca_topic_score_gemma":0.012156626,"teacher_disagreement_score":0.005971504,"about_ca_system_score_codex":0.00016268196,"about_ca_system_score_gemma":0.000107891836,"threshold_uncertainty_score":0.011873484},"labels":[],"label_agreement":null},{"id":"W2907642773","doi":"10.3847/1538-4357/ab2236","title":"The NANOGrav 11 yr Data Set: Limits on Gravitational Waves from Individual Supermassive Black Hole Binaries","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":153,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"","keywords":"Supermassive black hole; Gravitational wave; Pulsar; Galaxy; Observatory; Sky; Black hole (networking)","score_opus":0.033154132407057134,"score_gpt":0.3235139658769414,"score_spread":0.2903598334698843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2907642773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9751898,0.00011369373,0.0008930113,0.0001175563,0.000015208266,0.000023882556,0.02084043,0.000093871655,0.002712558],"genre_scores_gemma":[0.89860916,0.000075315234,0.0010186668,0.00007511539,0.000022219298,0.00003716904,0.099435866,0.00003298844,0.0006935824],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992329,0.000114656585,0.00011042095,0.00017323613,0.00027206732,0.00009668745],"domain_scores_gemma":[0.99647176,0.0011754059,0.00081443,0.0007785016,0.00039709866,0.0003628502],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013406351,0.00025131376,0.00042209384,0.0019421458,0.00042772456,0.0006833489,0.00056953426,0.00034072757,0.0015827655],"category_scores_gemma":[0.0041438225,0.0001751607,0.00030250754,0.00124574,0.00026521488,0.0005251139,0.0011707124,0.00024780704,0.0005836497],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005393705,0.00009909285,0.97477436,0.000044653956,0.00012520944,0.00018076214,0.00014581675,0.0047151614,0.002849425,0.00059156097,0.0053177285,0.010616821],"study_design_scores_gemma":[0.000059352238,0.0000638581,0.97816694,0.000017168875,0.00004238842,0.00014989839,0.000100394696,0.01158028,0.0024181053,0.0002306691,0.0071542575,0.000016701424],"about_ca_topic_score_codex":0.011912092,"about_ca_topic_score_gemma":0.018520152,"teacher_disagreement_score":0.011912092,"about_ca_system_score_codex":0.00037690403,"about_ca_system_score_gemma":0.00033242675,"threshold_uncertainty_score":0.023685455},"labels":[],"label_agreement":null},{"id":"W2907822564","doi":"10.3847/1538-4357/ab113b","title":"Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO<sup>*</sup>","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Ministry of Education, India; National Research Foundation of Korea; Engineering and Physical Sciences Research Council; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Kavli Foundation; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; Science and Engineering Research Board; National Science Foundation; Royal Society","keywords":"Neutron star; LIGO; Gravitational wave; Supernova; Exoplanet; Binary number; Amplitude; Binary star","score_opus":0.01123339613981883,"score_gpt":0.28611258537547263,"score_spread":0.2748791892356538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2907822564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985378,0.000077228506,0.00073046837,0.000015169998,0.0000017303752,0.000012384592,0.00015222076,0.000018153807,0.0004547869],"genre_scores_gemma":[0.99652666,0.000027561658,0.002695455,0.00001737775,0.0000049137407,0.000007630121,0.000622843,0.00000435634,0.00009323722],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996182,0.00011585215,0.00004333726,0.00008641111,0.00007018343,0.00006597312],"domain_scores_gemma":[0.9983279,0.0006075644,0.0004410255,0.00020306616,0.000094597046,0.00032583158],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001019228,0.00025088043,0.00024756757,0.0010331415,0.00027277184,0.00055144646,0.0003207126,0.000282008,0.0006504045],"category_scores_gemma":[0.0023076115,0.00013129895,0.00029936852,0.0006552978,0.00045717382,0.00026163945,0.0008058724,0.00022028458,0.00015135651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007197808,0.00008689337,0.9583776,0.000037005866,0.00019428041,0.00028858773,0.00023167123,0.0016169227,0.019635366,0.000331588,0.00017640828,0.01830384],"study_design_scores_gemma":[0.00006450542,0.0005362592,0.97913915,0.000014152186,0.00016052618,0.0008436251,0.00024879337,0.0040762145,0.012276628,0.0005241335,0.0020901756,0.000025958261],"about_ca_topic_score_codex":0.0019278445,"about_ca_topic_score_gemma":0.006078839,"teacher_disagreement_score":0.0019278445,"about_ca_system_score_codex":0.00026670206,"about_ca_system_score_gemma":0.00031508433,"threshold_uncertainty_score":0.005390227},"labels":[],"label_agreement":null},{"id":"W2907982033","doi":"10.3847/1538-4357/ab4185","title":"Host Galaxies of Type Ic and Broad-lined Type Ic Supernovae from the Palomar Transient Factory: Implications for Jet Production","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Smithsonian Astrophysical Observatory; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Israel Science Foundation; Lawrence Berkeley National Laboratory; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Ministerio de Ciencia, Tecnología e Innovación Productiva; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; W. M. Keck Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Supernova; Galaxy; Sky; Jet (fluid); Metallicity; Type (biology); Star formation; Transient (computer programming)","score_opus":0.02793259907737698,"score_gpt":0.24849631760244278,"score_spread":0.22056371852506582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2907982033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992962,0.000037069454,0.00005844856,0.000009859914,0.0000011480904,0.0000021865567,0.00023198215,0.0000070423903,0.00035606843],"genre_scores_gemma":[0.999511,0.0000169117,0.000047391466,0.0000055463515,0.000002271352,0.0000017818767,0.00033238958,0.000002677093,0.00008011665],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998312,0.000022176837,0.000014699331,0.0000644782,0.000026889333,0.000040484756],"domain_scores_gemma":[0.9988147,0.00019364776,0.00049555063,0.00012324307,0.00013558961,0.00023729276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003804871,0.00026829887,0.00028333446,0.0017849725,0.00030602067,0.0009316328,0.00027450858,0.00018989133,0.0024487972],"category_scores_gemma":[0.00077094487,0.00012614336,0.00021912194,0.0008496143,0.00037437087,0.00037086642,0.00064368744,0.0001995306,0.00034478153],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004671709,0.000009157729,0.99663526,0.0000044968815,0.000017098157,0.00009562706,0.00009181135,0.000025404486,0.0017089281,0.00002151649,0.000038291208,0.001305704],"study_design_scores_gemma":[0.0000017659723,0.00001727341,0.9993517,0.0000013900884,0.0000056606154,0.00015618591,0.00016374027,0.00006634534,0.0001581132,0.000012700967,0.00006404394,0.0000010487454],"about_ca_topic_score_codex":0.004388893,"about_ca_topic_score_gemma":0.0036928095,"teacher_disagreement_score":0.004388893,"about_ca_system_score_codex":0.00025886783,"about_ca_system_score_gemma":0.00012710072,"threshold_uncertainty_score":0.008726716},"labels":[],"label_agreement":null},{"id":"W2908719355","doi":"10.3847/1538-4357/aaff5c","title":"The Rotation-disk Connection in Young Brown Dwarfs: Strong Evidence for Early Rotational Braking","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; York University","funders":"Science and Technology Facilities Council","keywords":"Brown dwarf; Astrophysics; Rotation period; Physics; Stars; Rotation (mathematics); Light curve; Astronomy; Period (music); Geometry; Mathematics","score_opus":0.022863736312244937,"score_gpt":0.2715523127633605,"score_spread":0.24868857645111556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2908719355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995596,0.000046150773,0.000033063283,0.00000409704,7.4495256e-7,8.895972e-7,0.000054890403,0.000003383217,0.00029719746],"genre_scores_gemma":[0.99975735,0.000015831041,0.000037035454,0.0000027525682,0.0000023834377,5.9428345e-7,0.00009167553,0.0000013089115,0.000091067646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.00001409368,0.000012768851,0.000032526026,0.00002742874,0.000030968815],"domain_scores_gemma":[0.9985266,0.0002542459,0.0006079884,0.00010884385,0.00016525507,0.0003370248],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027630222,0.00015594666,0.00018720869,0.0011455303,0.00026798976,0.00051592913,0.00014296865,0.00016607791,0.0011514396],"category_scores_gemma":[0.0010359688,0.00010458735,0.0001054337,0.0005670605,0.0003889359,0.00020907696,0.00035467313,0.00012097231,0.0003093663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000086062646,0.000012934036,0.9919308,0.000009204578,0.000010561035,0.00012786587,0.0001418883,0.000036245736,0.005025225,0.00002263304,0.000028405902,0.0025681348],"study_design_scores_gemma":[6.544482e-7,0.00001954305,0.9994956,8.43634e-7,0.0000023160771,0.00014976769,0.0000492431,0.000028757342,0.00019017477,0.000010722002,0.0000516466,7.336556e-7],"about_ca_topic_score_codex":0.0022028962,"about_ca_topic_score_gemma":0.003703579,"teacher_disagreement_score":0.0022028962,"about_ca_system_score_codex":0.00017516538,"about_ca_system_score_gemma":0.00014585422,"threshold_uncertainty_score":0.004380107},"labels":[],"label_agreement":null},{"id":"W2908897897","doi":"10.3847/1538-4357/aaf50a","title":"High-redshift Massive Quiescent Galaxies Are as Flat as Star-forming Galaxies: The Flattening of Galaxies and the Correlation with Structural Properties in CANDELS/3D-HST","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Flattening; Galaxy; Elliptical galaxy; Peculiar galaxy; Luminous infrared galaxy; Lenticular galaxy; Radio galaxy; Galaxy formation and evolution","score_opus":0.005170378816995073,"score_gpt":0.18689320500560766,"score_spread":0.18172282618861257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2908897897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983797,0.000053709067,0.00013281716,0.000016261487,0.0000013619706,0.000002020324,0.0007954767,0.000034421333,0.00058423454],"genre_scores_gemma":[0.99850583,0.000012982933,0.00008560404,0.000008257232,0.000004286506,0.0000013340587,0.001240978,0.00000655623,0.00013418192],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997578,0.000018790266,0.000019397883,0.000075456024,0.000057262463,0.000071286384],"domain_scores_gemma":[0.9959466,0.000609652,0.0014489684,0.00050048897,0.00045261526,0.0010418231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005999371,0.0002140577,0.00026882454,0.0015348683,0.00032615426,0.0010358321,0.0003296762,0.00022526679,0.0022076534],"category_scores_gemma":[0.002351676,0.00016914685,0.00030812237,0.0009987069,0.0005570833,0.00049720565,0.00083833997,0.00031247846,0.0005962555],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040088056,0.0000067257415,0.9972881,0.0000036288536,0.000024649155,0.000015310483,0.000041792417,0.00018364741,0.0009248156,0.00003979882,0.00008907344,0.0013423215],"study_design_scores_gemma":[5.356182e-7,0.00000401123,0.9997445,5.138077e-7,0.0000013129927,0.000010077367,0.000024196235,0.000094963645,0.000065901906,0.000013077909,0.000040030696,9.685658e-7],"about_ca_topic_score_codex":0.0062728594,"about_ca_topic_score_gemma":0.008849818,"teacher_disagreement_score":0.0062728594,"about_ca_system_score_codex":0.0002235604,"about_ca_system_score_gemma":0.00014158864,"threshold_uncertainty_score":0.012472689},"labels":[],"label_agreement":null},{"id":"W2909005732","doi":"10.3847/1538-4357/aaf6b9","title":"The Fundamental Plane of Black Hole Accretion and Its Use as a Black Hole-Mass Estimator","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Black hole (networking); Accretion (finance); Intermediate-mass black hole; Accretion disc; Stellar black hole; Spin-flip; Fundamental plane (elliptical galaxies); Astronomy; Stars; Star formation; Galaxy","score_opus":0.01477114734920922,"score_gpt":0.24209829825050852,"score_spread":0.2273271509012993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909005732","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7394264,0.00052350806,0.25558892,0.00032785925,0.000019863124,0.000036214355,0.0008948406,0.00064746634,0.0025350468],"genre_scores_gemma":[0.97018313,0.00014860972,0.028388374,0.000036083246,0.000031962132,0.00002296055,0.0008132443,0.00009955904,0.00027616177],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99883395,0.0006867231,0.00003456387,0.00017196557,0.00018436162,0.00008854132],"domain_scores_gemma":[0.96958816,0.024119813,0.002407957,0.002349101,0.0010442928,0.0004906943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0059748306,0.00042786732,0.0006053786,0.0020735709,0.0005350217,0.0016889009,0.0008003379,0.00063742785,0.002053935],"category_scores_gemma":[0.03770094,0.00031595395,0.0006352863,0.00081885885,0.0015553582,0.001384372,0.0010231165,0.0008682131,0.00031345684],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000494037,0.000116886695,0.4008757,0.00011017957,0.00031447614,0.00026503325,0.0003861798,0.4373865,0.004748014,0.090970136,0.0024091233,0.061923645],"study_design_scores_gemma":[0.000017341315,0.00003790257,0.031925865,0.000029546067,0.000017800869,0.00010604158,0.00004674392,0.9461716,0.0013002967,0.019556357,0.0007700287,0.000020437115],"about_ca_topic_score_codex":0.005127201,"about_ca_topic_score_gemma":0.0021506636,"teacher_disagreement_score":0.0059748306,"about_ca_system_score_codex":0.0009455807,"about_ca_system_score_gemma":0.00087323115,"threshold_uncertainty_score":0.03159827},"labels":[],"label_agreement":null},{"id":"W2909133871","doi":"10.3847/1538-4357/aaf732","title":"The Size, Shape, and Scattering of Sagittarius A* at 86 GHz: First VLBI with ALMA","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":121,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"National Institutes of Natural Sciences; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Japan Society for the Promotion of Science; Recruitment Program of Global Experts; National Astronomical Observatory of Japan; National Research Foundation; National Research Foundation of Korea; Gordon and Betty Moore Foundation; John Templeton Foundation; Swinburne University of Technology; National Radio Astronomy Observatory; Harvard University; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Very-long-baseline interferometry; Sagittarius A*; Astrophysics; Supermassive black hole; Millimeter; Submillimeter Array; Galactic Center; Very Long Baseline Array; Astronomy; Angular diameter; Scattering; Schwarzschild radius; Angular resolution (graph drawing); Event horizon; Accretion (finance); Interstellar medium; Stars; Star formation; Active galactic nucleus; Galaxy; Optics; Event (particle physics)","score_opus":0.006166982070880004,"score_gpt":0.19504774498400992,"score_spread":0.1888807629131299,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909133871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98140967,0.00056366285,0.0061312653,0.0003738352,0.00003486605,0.000043113607,0.0017523268,0.00040566677,0.0092855925],"genre_scores_gemma":[0.98914844,0.00009626264,0.0072088935,0.00014220361,0.000055998487,0.000015172898,0.0022201482,0.00007340484,0.0010393917],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970067,0.000038450067,0.000008640698,0.00007089465,0.00010165364,0.00007961084],"domain_scores_gemma":[0.9994941,0.000047447822,0.00007000974,0.0000982749,0.00013271748,0.00015741996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006479803,0.0003771763,0.00041279162,0.001416458,0.00066504435,0.0011208742,0.00048572195,0.0005435577,0.0010701118],"category_scores_gemma":[0.0005522381,0.00041526588,0.00052197947,0.0006607657,0.00026043662,0.000401548,0.0009343406,0.0006818963,0.0006551669],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010798803,0.0006660244,0.5757806,0.00015360603,0.0006911375,0.0013832179,0.0014791582,0.0068227374,0.31922165,0.002903677,0.007669225,0.08214911],"study_design_scores_gemma":[0.000033708802,0.00016683366,0.96364504,0.000040739018,0.00011202616,0.00045744807,0.00020633,0.012065019,0.011801624,0.0005661276,0.010863842,0.00004119884],"about_ca_topic_score_codex":0.008624194,"about_ca_topic_score_gemma":0.015538695,"teacher_disagreement_score":0.008624194,"about_ca_system_score_codex":0.0008343458,"about_ca_system_score_gemma":0.00034802052,"threshold_uncertainty_score":0.017148018},"labels":[],"label_agreement":null},{"id":"W2909168123","doi":"10.3847/1538-4357/ab09ec","title":"Weak Shock Propagation with Accretion. II. Stability of Self-similar Solutions to Radial Perturbations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Eagle Ridge Hospital","funders":"Gordon and Betty Moore Foundation","keywords":"Shock wave; Formalism (music); Perturbation (astronomy); Shock (circulatory); Stability (learning theory); Radial velocity; Gravitation; Gravitational field","score_opus":0.0108858849545188,"score_gpt":0.21464558384065327,"score_spread":0.20375969888613446,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909168123","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9171857,0.0003194817,0.07305632,0.00045378157,0.000055603065,0.00007717748,0.00005383265,0.00019681384,0.008601211],"genre_scores_gemma":[0.9951486,0.00006239737,0.0029962882,0.00005859243,0.000019664245,0.0000206906,0.000021707649,0.000015952606,0.0016561308],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998609,0.000033619588,0.000011612637,0.000024356494,0.000037650716,0.000031908105],"domain_scores_gemma":[0.9993168,0.0001477393,0.00029040547,0.000060200186,0.00011185402,0.00007292167],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039920493,0.00040464944,0.0003363406,0.00064723386,0.0005848143,0.00092892995,0.0006243269,0.0009063917,0.00096338027],"category_scores_gemma":[0.002373595,0.0002970862,0.00066424056,0.00018669637,0.0010937685,0.0008544771,0.0010110943,0.00061209383,0.00021683908],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030685685,0.0001681642,0.017738873,0.0001940382,0.0002002698,0.0014070296,0.0009573533,0.58658683,0.16141768,0.21473326,0.0015550355,0.014734688],"study_design_scores_gemma":[0.00002515903,0.00003947704,0.0018883143,0.000008468686,0.000007822252,0.000103324695,0.000060392063,0.97954434,0.0060810787,0.011804301,0.00042038003,0.000016928983],"about_ca_topic_score_codex":0.0016538855,"about_ca_topic_score_gemma":0.00046625413,"teacher_disagreement_score":0.0016538855,"about_ca_system_score_codex":0.00086191966,"about_ca_system_score_gemma":0.00035079493,"threshold_uncertainty_score":0.0062536597},"labels":[],"label_agreement":null},{"id":"W2909193581","doi":"10.3847/1538-4357/ab2892","title":"Memoirs of a Giant Planet","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration","keywords":"Planet; Jovian; Saturn; Dissipation; Jupiter (rocket family); Giant planet; Amplitude; Gas giant","score_opus":0.004849263969120047,"score_gpt":0.19059780170555915,"score_spread":0.1857485377364391,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909193581","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.06857431,0.040608883,0.003960135,0.29803345,0.094281495,0.00005901104,0.0018191716,0.00045986302,0.4922036],"genre_scores_gemma":[0.671787,0.012990977,0.0016478775,0.040326048,0.02865837,0.00005907571,0.000544564,0.0003343919,0.2436517],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996792,0.00015094846,0.000011335547,0.000060263723,0.000060113915,0.000038167385],"domain_scores_gemma":[0.9990945,0.00048056972,0.000082675666,0.00009635963,0.00011757408,0.00012835806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068894256,0.00036556143,0.00020039696,0.0005131238,0.0021491272,0.0019420063,0.00040557398,0.0013193727,0.011037764],"category_scores_gemma":[0.003244273,0.00011711115,0.00020857084,0.00026213683,0.0032854492,0.0022298936,0.0013535467,0.0022702655,0.002090005],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026405088,0.000033338376,0.002677172,0.00067136163,0.00006257561,0.0042871507,0.05504997,0.00026679493,0.0035335128,0.161376,0.7286941,0.043084085],"study_design_scores_gemma":[0.000005899451,0.000022494281,0.0007124418,0.00012048827,0.0000058673513,0.00087935355,0.0039412207,0.00008683097,0.0004477756,0.007161855,0.98660755,0.000008188108],"about_ca_topic_score_codex":0.0012052153,"about_ca_topic_score_gemma":0.0022216411,"teacher_disagreement_score":0.011037764,"about_ca_system_score_codex":0.00110353,"about_ca_system_score_gemma":0.0003161417,"threshold_uncertainty_score":0.036925018},"labels":[],"label_agreement":null},{"id":"W2909963127","doi":"10.3847/1538-4357/aafd31","title":"Protoplanetary Disk Rings and Gaps across Ages and Luminosities","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":153,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Planetesimal; Astrophysics; Physics; Planet; RADIUS; Radiative transfer; Stars; Astronomy; Snow line; Clearance; Protoplanetary disk; Snow","score_opus":0.005394852583008965,"score_gpt":0.2265937394604339,"score_spread":0.22119888687742495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2909963127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991611,0.000102227605,0.00004569591,0.0000031750328,4.7914165e-7,0.000001967777,0.0002793547,0.000006545259,0.00039951096],"genre_scores_gemma":[0.99950504,0.000028156,0.00007305075,0.0000014431904,0.0000012436369,0.0000017800621,0.00019534859,0.0000018083061,0.00019204563],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997832,0.000032459342,0.00001687401,0.000078604426,0.000039222097,0.000049586015],"domain_scores_gemma":[0.99814725,0.00037063792,0.0008323705,0.0002005332,0.0002495828,0.00019964892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002960782,0.00014103914,0.00014273587,0.0017753375,0.000247641,0.00059682375,0.00022595258,0.0001574226,0.00200656],"category_scores_gemma":[0.0010513404,0.000089384026,0.00013085961,0.0007674756,0.0002630346,0.00042596782,0.00051250285,0.00009157256,0.0004196301],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016411497,0.000023814624,0.9881721,0.000018300865,0.000023553837,0.00010170004,0.00041635783,0.0001968223,0.00399198,0.00009266953,0.00009359821,0.006705003],"study_design_scores_gemma":[0.0000013277204,0.000029868825,0.99859554,0.0000028712745,0.000007609228,0.00015217818,0.00021927434,0.00014741093,0.00053256616,0.00003580317,0.00027386978,0.0000016680715],"about_ca_topic_score_codex":0.0014687337,"about_ca_topic_score_gemma":0.0018471772,"teacher_disagreement_score":0.00200656,"about_ca_system_score_codex":0.00018659137,"about_ca_system_score_gemma":0.00008032457,"threshold_uncertainty_score":0.0067126155},"labels":[],"label_agreement":null},{"id":"W2910012994","doi":"10.3847/1538-4357/aafac2","title":"The Temporal Requirements of Directly Observing Self-gravitating Spiral Waves in Protoplanetary Disks with ALMA","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Substructure; Radiative transfer; Spiral galaxy; Accretion disc; Spiral (railway); Accretion (finance); Gravitational instability; Planetary system","score_opus":0.013635680400374797,"score_gpt":0.24609730967135846,"score_spread":0.23246162927098366,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2910012994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864477,0.000028990904,0.00064929517,0.00005328375,0.0000027977565,0.0000036822244,0.000062107625,0.000033504355,0.00052154076],"genre_scores_gemma":[0.99957806,0.000006461997,0.00028501486,0.000007985721,0.0000016660337,0.0000031687875,0.00006359366,0.0000043811624,0.00004958558],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998381,0.000035451907,0.000008439492,0.00004524291,0.00003367491,0.000038929327],"domain_scores_gemma":[0.9972988,0.0018318741,0.0003304532,0.00017435063,0.00015360233,0.0002108818],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066716055,0.0002357435,0.00026721033,0.0002686137,0.00050125044,0.0007648523,0.00064351386,0.000529637,0.0014740553],"category_scores_gemma":[0.0055169864,0.00028467015,0.0004000123,0.0001938546,0.0003892304,0.0006220333,0.00057176704,0.00046646662,0.00010942446],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009053143,0.00034074474,0.74554265,0.000108676046,0.00025510043,0.0006322117,0.0002640886,0.19070412,0.048672955,0.002633286,0.000375901,0.009565002],"study_design_scores_gemma":[0.000122063335,0.00037652857,0.24912472,0.000018555502,0.00011544575,0.00025246324,0.00022288771,0.7384401,0.00926315,0.0015099153,0.00051433855,0.00003979742],"about_ca_topic_score_codex":0.0062040254,"about_ca_topic_score_gemma":0.0061434815,"teacher_disagreement_score":0.0062040254,"about_ca_system_score_codex":0.0006703227,"about_ca_system_score_gemma":0.00038256386,"threshold_uncertainty_score":0.012335837},"labels":[],"label_agreement":null},{"id":"W2910884839","doi":"10.3847/1538-4357/aaf723","title":"Erratum: “Can We Distinguish Low-mass Black Holes in Neutron Star Binaries?” (2018, ApJ, 856, 110)","year":2019,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Mechanics and Biomechanics Studies","field":"Engineering","cited_by":16,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Physics; Neutron star; Astrophysics; Star (game theory); Astronomy","score_opus":0.010548257760055113,"score_gpt":0.20487851350477804,"score_spread":0.19433025574472293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2910884839","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00046503337,0.000992127,0.0002813373,0.06851215,0.9214413,0.000014982097,0.0012935901,0.00023560453,0.0067637796],"genre_scores_gemma":[0.021479763,0.0069121527,0.0038749378,0.17194423,0.4461988,0.000121487574,0.0059063775,0.0016440639,0.34191814],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99846894,0.00019773998,0.0003172858,0.00025281322,0.0006213469,0.00014187164],"domain_scores_gemma":[0.9900889,0.0026926904,0.0007559432,0.00068744784,0.005002528,0.00077260664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002210341,0.001876557,0.0012452162,0.003027308,0.0046359366,0.0032740096,0.0022545604,0.0057923933,0.053850904],"category_scores_gemma":[0.028286945,0.0006885087,0.001109269,0.0015870989,0.002269947,0.0028286264,0.0020552687,0.008123875,0.037617497],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030170546,0.00000685434,0.00012685871,0.000046463676,0.0000050722965,0.00016526208,0.000023701263,0.000018952369,0.000053385396,0.0007471082,0.99595165,0.0028245319],"study_design_scores_gemma":[0.0000436586,0.000039425824,0.0026414567,0.00034435798,0.000039154245,0.0006672807,0.00029865245,0.00021840422,0.00041323723,0.00601351,0.98922193,0.000058750917],"about_ca_topic_score_codex":0.014203378,"about_ca_topic_score_gemma":0.01644081,"teacher_disagreement_score":0.053850904,"about_ca_system_score_codex":0.0026218349,"about_ca_system_score_gemma":0.0033043127,"threshold_uncertainty_score":0.1801492},"labels":[],"label_agreement":null},{"id":"W2911381628","doi":"10.3847/1538-4357/ab05e2","title":"Changing-look Quasar Candidates: First Results from Follow-up Spectroscopy of Highly Optically Variable Quasars","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Max-Planck-Gesellschaft; Chinese Academy of Sciences; Queen's University Belfast; Durham University; York University; Space Telescope Science Institute; Science and Technology Facilities Council; Universität Basel; Fermilab; National Science Foundation; Case Western Reserve University; Carnegie Mellon University; University of Pittsburgh; Los Alamos National Laboratory; College of Engineering, Michigan State University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Queen's University; Harvard University; Ohio State University; Vanderbilt University; Drexel University; U.S. Naval Observatory; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Science Mission Directorate; Yale University","keywords":"Quasar; Sky; Photometry (optics); Spectroscopy; Spectral line; Active galactic nucleus","score_opus":0.005734780925599284,"score_gpt":0.2028296293542577,"score_spread":0.1970948484286584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2911381628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986595,0.00012689283,0.00020706658,0.0000208599,0.0000029129917,0.000022192375,0.00039946352,0.000008746383,0.0005524411],"genre_scores_gemma":[0.9987023,0.000052226613,0.00028867112,0.00003330825,0.00000766564,0.000007304838,0.0007274022,0.0000046583486,0.00017644008],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99950075,0.00007560789,0.000029025276,0.00015198486,0.00012211756,0.00012039422],"domain_scores_gemma":[0.9973647,0.00055467803,0.0005206788,0.0003183781,0.00063496275,0.0006065465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00073883013,0.00021671756,0.00023422377,0.0014324002,0.0005396923,0.0006775754,0.00043808442,0.00039650753,0.00080178445],"category_scores_gemma":[0.0015928631,0.0001456709,0.00026517946,0.0005361144,0.00025846928,0.00027791117,0.0008117209,0.00030563874,0.00039815766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005677842,0.00005375355,0.9943433,0.00000706543,0.000016015545,0.00024894532,0.00016760165,0.000028433036,0.0022710667,0.000012568134,0.00010286049,0.0026915933],"study_design_scores_gemma":[0.0000027444987,0.00007538539,0.9988029,0.0000033367483,0.000016777913,0.00031092874,0.00017519105,0.000092230046,0.00028919126,0.000010063767,0.00021863676,0.0000027150866],"about_ca_topic_score_codex":0.0065614763,"about_ca_topic_score_gemma":0.011919064,"teacher_disagreement_score":0.0065614763,"about_ca_system_score_codex":0.00023086391,"about_ca_system_score_gemma":0.00017758268,"threshold_uncertainty_score":0.013046563},"labels":[],"label_agreement":null},{"id":"W2911391557","doi":"10.3847/1538-4357/ab02fe","title":"Source Structure and Molecular Gas Properties from High-resolution CO Imaging of SPT-selected Dusty Star-forming Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Submillimeter Array; Millimeter; Astronomy; Star formation; Line (geometry); Dust lane; Luminous infrared galaxy; Interstellar medium; Geometry","score_opus":0.004539939474123221,"score_gpt":0.19170225309040947,"score_spread":0.18716231361628624,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2911391557","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992673,0.000022713582,0.00025533294,0.000007993445,6.078638e-7,0.000002465328,0.00014600498,0.000018861692,0.0002787419],"genre_scores_gemma":[0.9993736,0.000008374045,0.00026095772,0.000004039672,0.0000029360306,0.0000014297666,0.00031287133,0.0000032067442,0.000032504056],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985063,0.000016567195,0.000010990465,0.00004637642,0.00004962465,0.000025874053],"domain_scores_gemma":[0.99923754,0.000118649805,0.00027464473,0.00008083,0.0001323002,0.00015600983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002485479,0.00016994061,0.00019342257,0.0012743494,0.00022814768,0.00050480536,0.00027426684,0.0002486548,0.0006881075],"category_scores_gemma":[0.0008029217,0.00016197769,0.0002350587,0.0006804632,0.00021740053,0.00026552886,0.00041277194,0.00016411392,0.00019348324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011307823,0.000032754164,0.964336,0.000019976595,0.00007286995,0.0001720584,0.00018006784,0.001429316,0.028835576,0.00006604998,0.00016580909,0.004576586],"study_design_scores_gemma":[0.000002989448,0.000018396224,0.9964958,0.0000012686121,0.000010118874,0.00007034402,0.000046857385,0.0023459983,0.000921813,0.000014612704,0.00007005127,0.0000018254864],"about_ca_topic_score_codex":0.004489403,"about_ca_topic_score_gemma":0.0061868154,"teacher_disagreement_score":0.004489403,"about_ca_system_score_codex":0.00036239068,"about_ca_system_score_gemma":0.000081021004,"threshold_uncertainty_score":0.008926511},"labels":[],"label_agreement":null},{"id":"W2911700471","doi":"10.3847/1538-4357/ab0e8f","title":"Low-latency Gravitational-wave Alerts for Multimessenger Astronomy during the Second Advanced LIGO and Virgo Observing Run","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council; Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Division of Human Resource Development; Indian Institute of Science Education and Research Mohali; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Ministry of Education, India; National Research Foundation of Korea; Engineering and Physical Sciences Research Council; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Kavli Foundation; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Université de Lyon; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; Science and Engineering Research Board; National Science Foundation; Royal Society","keywords":"LIGO; Gravitational wave; Physics; Neutron star; Astronomy; Gravitational-wave astronomy; Astrophysics; Gravitational-wave observatory","score_opus":0.009292788840362914,"score_gpt":0.27264479551870596,"score_spread":0.263352006678343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2911700471","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96732485,0.0003698877,0.0038767396,0.0007253116,0.00024205394,0.00030172747,0.007287857,0.005632157,0.01423946],"genre_scores_gemma":[0.9807304,0.00011596873,0.003835529,0.00032894942,0.00022115727,0.00014031053,0.010633875,0.00033382038,0.0036599764],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9985102,0.00015665412,0.00006306804,0.00026013693,0.0005472837,0.00046258204],"domain_scores_gemma":[0.9963593,0.0005588538,0.0007940933,0.00043243065,0.0006122742,0.0012430252],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001614491,0.00048664212,0.00031725373,0.0021283086,0.0007905535,0.001601584,0.00044387786,0.0005940367,0.0032555691],"category_scores_gemma":[0.0049187234,0.00019745238,0.00027519697,0.0012113826,0.00024275026,0.00082060666,0.0027775748,0.00079200685,0.0018440894],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019794714,0.00056868186,0.7655493,0.00024192892,0.00018141686,0.0016783542,0.0030790728,0.0019084287,0.023978993,0.0017231668,0.05803679,0.14107445],"study_design_scores_gemma":[0.000098134056,0.00039604524,0.9059868,0.00009171418,0.000075677075,0.0004964996,0.0013352934,0.006472927,0.0066678193,0.0007924732,0.07750346,0.00008317607],"about_ca_topic_score_codex":0.0057763318,"about_ca_topic_score_gemma":0.006923413,"teacher_disagreement_score":0.0057763318,"about_ca_system_score_codex":0.00071809447,"about_ca_system_score_gemma":0.0009223581,"threshold_uncertainty_score":0.011485457},"labels":[],"label_agreement":null},{"id":"W2911969062","doi":"10.3847/1538-4357/ab77aa","title":"The MBHBM<sub>⋆</sub> Project. I. Measurement of the Central Black Hole Mass in Spiral Galaxy NGC 3504 Using Molecular Gas Kinematics","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Supermassive black hole; Galaxy; Submillimeter Array; Barred spiral galaxy; Black hole (networking); Spiral galaxy; Milky Way; Astronomy; Elliptical galaxy; Interacting galaxy; Star formation","score_opus":0.01782163359426292,"score_gpt":0.21609109926529518,"score_spread":0.19826946567103226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2911969062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96197283,0.0005506253,0.006481712,0.0003381482,0.000030001385,0.00032136627,0.016329201,0.001130132,0.012845925],"genre_scores_gemma":[0.94182277,0.0001474011,0.02665564,0.0001267217,0.00002613063,0.00022770415,0.027459102,0.000090886555,0.0034437021],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996511,0.00009062792,0.000012461939,0.000060111248,0.00012597784,0.000059745646],"domain_scores_gemma":[0.9993311,0.000049694932,0.00013307147,0.00010081432,0.00012508649,0.00026022867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009947707,0.00041042577,0.00013712955,0.0012469331,0.000282136,0.00038705504,0.00040747307,0.00026952155,0.0018488043],"category_scores_gemma":[0.00054506934,0.00012183001,0.00015924196,0.0005067852,0.00025935203,0.0002858241,0.0007174139,0.00012115553,0.0007173133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014701149,0.0005085843,0.7468114,0.00009550367,0.00018023992,0.00032441193,0.00036517615,0.0028047494,0.0960683,0.002703688,0.014571693,0.13409612],"study_design_scores_gemma":[0.00010265278,0.0007321488,0.93660605,0.00001851826,0.00004775756,0.00027732644,0.00015728787,0.0057322904,0.03193605,0.00065929565,0.02371413,0.00001647488],"about_ca_topic_score_codex":0.007902605,"about_ca_topic_score_gemma":0.009161616,"teacher_disagreement_score":0.007902605,"about_ca_system_score_codex":0.00048459746,"about_ca_system_score_gemma":0.00033497342,"threshold_uncertainty_score":0.015713215},"labels":[],"label_agreement":null},{"id":"W2911977857","doi":"10.3847/1538-4357/ab053e","title":"The Occurrence of Compact Groups of Galaxies through Cosmic Time","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; Western University","funders":"","keywords":"Galaxy; Galaxy group; Population; Luminous infrared galaxy; Redshift; Galaxy formation and evolution; Lenticular galaxy; Elliptical galaxy","score_opus":0.007815111157584749,"score_gpt":0.22034812660954736,"score_spread":0.21253301545196263,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2911977857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994724,0.000052147563,0.0030007209,0.00008774096,0.0000043774353,0.000008580712,0.00067217083,0.00014201402,0.00130819],"genre_scores_gemma":[0.9975821,0.000025088473,0.0014860624,0.0000116214605,0.000002538732,0.000010843069,0.0005907975,0.000029472381,0.00026150473],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9997769,0.0000580303,0.000008333503,0.00007346345,0.00004856925,0.000034604713],"domain_scores_gemma":[0.9980546,0.0008464762,0.0003969598,0.0003024162,0.00016459466,0.00023499787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00091139803,0.00026536055,0.00034746208,0.0008658094,0.0003149567,0.0014020858,0.0008347219,0.00037628438,0.0021811384],"category_scores_gemma":[0.006044522,0.00029558883,0.0005471376,0.00069393666,0.00059278,0.00080373045,0.0007844417,0.0004196671,0.00020196971],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002503323,0.00007542005,0.45851836,0.0000435054,0.00026572502,0.00017336216,0.0003470318,0.5167696,0.0021802143,0.010793622,0.0012728676,0.009310056],"study_design_scores_gemma":[0.00004333964,0.000058069236,0.07015712,0.000012713963,0.000045310448,0.00009456712,0.00008432771,0.9227198,0.0009333333,0.004982061,0.00084224273,0.0000272137],"about_ca_topic_score_codex":0.010162191,"about_ca_topic_score_gemma":0.0047700424,"teacher_disagreement_score":0.010162191,"about_ca_system_score_codex":0.00070799177,"about_ca_system_score_gemma":0.00034727494,"threshold_uncertainty_score":0.020206094},"labels":[],"label_agreement":null},{"id":"W2912154889","doi":"10.3847/1538-4357/ab04f7","title":"Quenching Low-mass Satellite Galaxies: Evidence for a Threshold ICM Density","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McMaster University","funders":"","keywords":"Ram pressure; Quenching (fluorescence); Galaxy; Intracluster medium; Cluster (spacecraft); Galaxy cluster; Sky","score_opus":0.016105282570403986,"score_gpt":0.24547050085596434,"score_spread":0.22936521828556033,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912154889","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917406,0.0000912719,0.0002234798,0.000012339179,5.4610706e-7,0.0000018508883,0.00014796507,0.000027334187,0.00032109543],"genre_scores_gemma":[0.9998092,0.000010546012,0.000044349377,0.0000051675634,9.955074e-7,7.826819e-7,0.000092648166,0.000002434396,0.000034020908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997745,0.000023519897,0.000012694907,0.00008351149,0.000058434453,0.00004735918],"domain_scores_gemma":[0.9979006,0.00042485757,0.00076918345,0.00032513757,0.00023942176,0.00034077634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029026074,0.00012915999,0.0003770381,0.00077862595,0.00024848417,0.00054839614,0.00042412584,0.00018328005,0.0014537887],"category_scores_gemma":[0.0021697194,0.00016758498,0.00015404078,0.00056333485,0.0008188405,0.0003292048,0.0005218183,0.00021947657,0.00013794424],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000106518535,0.000014223765,0.9803745,0.00002462531,0.000041691783,0.00005955732,0.00018843921,0.0006723478,0.015783958,0.00032420905,0.000120014345,0.0022899308],"study_design_scores_gemma":[0.0000023676769,0.000020405325,0.9976439,0.0000020615528,0.000007872898,0.00005282109,0.000043480908,0.000766452,0.0012278059,0.00010777598,0.00012247587,0.0000024810793],"about_ca_topic_score_codex":0.0055846525,"about_ca_topic_score_gemma":0.004895595,"teacher_disagreement_score":0.0055846525,"about_ca_system_score_codex":0.0004557323,"about_ca_system_score_gemma":0.00014773334,"threshold_uncertainty_score":0.011104286},"labels":[],"label_agreement":null},{"id":"W2912207578","doi":"10.3847/1538-4357/aaf972","title":"Identifying Variability in Deeply Embedded Protostars with ALMA and CARMA","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Millimeter; Stars; Brightness; Accretion (finance); Serpens; Submillimeter Array; Interferometry; Astronomical interferometer","score_opus":0.008082170839845275,"score_gpt":0.2386660806012164,"score_spread":0.23058390976137114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912207578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995055,0.000029959892,0.00013748063,0.00000433309,0.0000014320406,0.0000017399941,0.000057674624,0.000006417,0.00025545398],"genre_scores_gemma":[0.99967337,0.0000065506633,0.00015328753,0.0000038901667,0.0000023150844,0.000001452751,0.00009951786,0.0000015576411,0.00005819481],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998222,0.000024594165,0.000013016759,0.00006624624,0.00003294096,0.000041116517],"domain_scores_gemma":[0.9991677,0.00015447215,0.0003049517,0.00012479557,0.000094635005,0.00015350233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029927318,0.00017254228,0.00021536053,0.0010405395,0.00022730719,0.0005311868,0.00023781773,0.0002307167,0.00070556055],"category_scores_gemma":[0.0010689512,0.00014236587,0.00018339368,0.00054256106,0.00026595805,0.00028600235,0.0006565452,0.00020486329,0.0001835247],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010808087,0.00002125401,0.97082776,0.0000066289244,0.00003913758,0.00012034534,0.00023195804,0.00015041835,0.025021255,0.00006432255,0.000045785888,0.0033629742],"study_design_scores_gemma":[0.0000010603508,0.000018916673,0.9989711,0.0000010124279,0.0000041261837,0.00008645529,0.00007194288,0.00018847012,0.00055624364,0.000015828462,0.000083779756,0.0000010418815],"about_ca_topic_score_codex":0.0013564851,"about_ca_topic_score_gemma":0.0033913867,"teacher_disagreement_score":0.0013564851,"about_ca_system_score_codex":0.00018533014,"about_ca_system_score_gemma":0.00007466587,"threshold_uncertainty_score":0.0026971698},"labels":[],"label_agreement":null},{"id":"W2912672882","doi":"10.3847/1538-4357/aaf8a9","title":"AstroSat SXT Observations of Her X-1","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Black-body radiation; Astrophysics; Spectral line; Emission spectrum; Telescope; Ionization; Corona (planetary geology); Line (geometry); Astronomy; Radiation; Ion; Optics","score_opus":0.017431450541452422,"score_gpt":0.23005488385942446,"score_spread":0.21262343331797204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912672882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99511117,0.000061953586,0.00008636741,0.000029453711,0.000004958861,0.000006290692,0.0011978028,0.00004347724,0.0034585418],"genre_scores_gemma":[0.9929929,0.00004451946,0.00046861367,0.000027896842,0.000016809361,0.000006024985,0.0040023997,0.000022828355,0.0024179758],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987113,0.000011042317,0.000004884192,0.000041936877,0.000044571087,0.000026452512],"domain_scores_gemma":[0.99973756,0.000020287627,0.000082702536,0.00004248126,0.00005941051,0.00005751843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025139426,0.00019625713,0.00024575417,0.0012067012,0.00042294632,0.00040867823,0.00018658374,0.00023329104,0.0027505725],"category_scores_gemma":[0.00024219933,0.0001510477,0.00015442698,0.0008308083,0.00018040999,0.00023516138,0.00049574266,0.00023139412,0.0007355483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017377331,0.00028992034,0.73897666,0.0001208244,0.00019686656,0.0016656404,0.0012032966,0.0018243045,0.21673313,0.0011273045,0.0052483804,0.030875964],"study_design_scores_gemma":[0.000027209517,0.00012066305,0.9911418,0.0000057990223,0.00001689068,0.00030002528,0.00010773032,0.0009142178,0.0034913647,0.00008308724,0.0037842984,0.0000068561817],"about_ca_topic_score_codex":0.003058629,"about_ca_topic_score_gemma":0.007969173,"teacher_disagreement_score":0.003058629,"about_ca_system_score_codex":0.00038275812,"about_ca_system_score_gemma":0.00011817427,"threshold_uncertainty_score":0.009201586},"labels":[],"label_agreement":null},{"id":"W2912673829","doi":"10.3847/1538-4357/ab0306","title":"A Wide-field Photometric Survey of Globular Clusters in the Peculiar Early-type Galaxy M85","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Globular cluster; Galaxy; Astrophysics; Effective radius; Luminosity; RADIUS; Astronomy","score_opus":0.009963685143064501,"score_gpt":0.22486011745188836,"score_spread":0.21489643230882385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912673829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99954045,0.000036317204,0.000044137272,0.000005918593,4.1806027e-7,0.0000021205558,0.0001483111,0.0000062711943,0.00021607887],"genre_scores_gemma":[0.9992673,0.000032466025,0.00015432588,0.000009391412,0.0000024942121,0.0000017366223,0.00039062547,0.0000015794689,0.0001400965],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998604,0.000016083213,0.000008321428,0.000043108237,0.000037070655,0.000035029843],"domain_scores_gemma":[0.9995839,0.00003282838,0.00011853223,0.000044732296,0.000063224965,0.00015676366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026008624,0.0001670169,0.00016828346,0.0016506833,0.0003420716,0.00031493147,0.00021626572,0.00017626566,0.00058183155],"category_scores_gemma":[0.00034642796,0.000112891204,0.00014393024,0.0010838474,0.00020683522,0.00018765173,0.00045685272,0.00009946542,0.00019346793],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004263662,0.000028700895,0.988192,0.000013644597,0.000029843954,0.000075159034,0.00037590446,0.0001268631,0.00544905,0.000060992894,0.0002940334,0.0053112363],"study_design_scores_gemma":[6.9512333e-7,0.00000807823,0.99965274,0.0000011357911,0.000003058108,0.000017396656,0.00005371092,0.000062482846,0.000056734636,0.000004258776,0.00013895263,6.54586e-7],"about_ca_topic_score_codex":0.01435334,"about_ca_topic_score_gemma":0.03216736,"teacher_disagreement_score":0.01435334,"about_ca_system_score_codex":0.0003129856,"about_ca_system_score_gemma":0.0001749167,"threshold_uncertainty_score":0.028539598},"labels":[],"label_agreement":null},{"id":"W2912945671","doi":"10.3847/1538-4357/aafb72","title":"Cosmic Pathways for Compact Groups in the Milli-Millennium Simulation","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; Canadian Space Agency; Western University","funders":"","keywords":"Galaxy; COSMIC cancer database; Galaxy formation and evolution; Star formation; Galaxy group; Compact group; Stellar mass; Cosmology; Universe","score_opus":0.013254962785976819,"score_gpt":0.22996681744685935,"score_spread":0.21671185466088252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912945671","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99648774,0.000056189543,0.0015526117,0.00013538057,0.0000053087365,0.0000066859134,0.000550755,0.00008980271,0.0011154317],"genre_scores_gemma":[0.99734855,0.000017661285,0.0014925704,0.000020565554,0.0000022232075,0.000010494385,0.00090781506,0.000025895695,0.00017418232],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998342,0.000049994058,0.0000057361094,0.00004774758,0.000026731963,0.00003568426],"domain_scores_gemma":[0.9991597,0.00024992178,0.00014342934,0.00013451329,0.00007250934,0.00023997226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007936096,0.00018571118,0.00024894637,0.00083946233,0.00051173475,0.00086672726,0.0006623341,0.00028730047,0.001744418],"category_scores_gemma":[0.0030752677,0.00022037384,0.00040714786,0.0006376557,0.0003121664,0.0005546406,0.00085796736,0.0004159955,0.00010860603],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003461765,0.000110990775,0.78319705,0.00005001859,0.000294817,0.000250943,0.00060941273,0.16408522,0.0032383977,0.028462468,0.0037376226,0.015616927],"study_design_scores_gemma":[0.00010899193,0.00009316282,0.31235212,0.000026104732,0.00009835357,0.00017333348,0.00033095755,0.66745514,0.0018722408,0.012699399,0.004730075,0.00006015227],"about_ca_topic_score_codex":0.012736804,"about_ca_topic_score_gemma":0.010900965,"teacher_disagreement_score":0.012736804,"about_ca_system_score_codex":0.0009245644,"about_ca_system_score_gemma":0.00040250132,"threshold_uncertainty_score":0.025325298},"labels":[],"label_agreement":null},{"id":"W2912971615","doi":"10.3847/1538-4357/ab0083","title":"A Sub-damped Lyα Absorber with Unusual Abundances: Evidence of Gas Recycling in a Low-redshift Galaxy Group","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Galaxy; Metallicity; Space Telescope Imaging Spectrograph; Interstellar medium; Galaxy group; Spectral line; Photoionization; Spectroscopy; Abundance of the chemical elements","score_opus":0.008980312954987434,"score_gpt":0.225323075147803,"score_spread":0.21634276219281556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2912971615","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99973387,0.00001472012,0.000054801734,0.0000058217897,4.008944e-7,0.000001228602,0.000014612213,0.0000046799382,0.00016991874],"genre_scores_gemma":[0.999754,0.000006726502,0.0000864912,0.000007771857,0.0000021535802,0.0000012635323,0.000041253417,0.0000017208869,0.00009852213],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991345,0.000008434093,0.0000053955705,0.000029123841,0.000017623446,0.000026028754],"domain_scores_gemma":[0.9995987,0.00003837541,0.00015164922,0.0000407111,0.00004336618,0.00012722808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017218316,0.00023497446,0.00026140705,0.0012106403,0.000424158,0.00046409422,0.00044911227,0.00031535063,0.0012848844],"category_scores_gemma":[0.0003156144,0.00015599783,0.00015893175,0.00046819774,0.00045407843,0.00020330287,0.00037561348,0.00018360277,0.00027143914],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000108488995,0.000062953266,0.9449955,0.000008282246,0.00003393581,0.0005786883,0.00038105182,0.00007454982,0.051349424,0.00008542509,0.00004875003,0.0022728648],"study_design_scores_gemma":[0.0000036108997,0.00006030041,0.9977725,0.0000012269543,0.000011269355,0.00048142162,0.00018037985,0.00036491893,0.00096831674,0.00004050332,0.000113160895,0.0000023900368],"about_ca_topic_score_codex":0.0030811103,"about_ca_topic_score_gemma":0.0030544405,"teacher_disagreement_score":0.0030811103,"about_ca_system_score_codex":0.00024774656,"about_ca_system_score_gemma":0.00008088607,"threshold_uncertainty_score":0.006126344},"labels":[],"label_agreement":null},{"id":"W2913016105","doi":"10.3847/1538-4357/ab2ada","title":"Investigation of Two Fermi-LAT Gamma-Ray Blazars Coincident with High-energy Neutrinos Detected by IceCube","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Istituto Nazionale di Fisica Nucleare; Chiba University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Natural Sciences and Engineering Research Council of Canada; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Knut och Alice Wallenbergs Stiftelse; Deutsches Elektronen-Synchrotron; Agenzia Spaziale Italiana; Chinese Academy of Sciences; Marsden Fund; Bundesministerium für Bildung und Forschung; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Western Canada Research Grid; Center for Cosmology and Astroparticle Physics, Ohio State University; National Research Foundation of Korea; Villum Fonden; High Energy Accelerator Research Organization; Ohio State University; National Research Foundation; Michigan State University; Compute Canada; Polarforskningssekretariatet; Ministry of Education, Culture, Sports, Science and Technology; Chinese Academy of Sciences South America Center for Astronomy; Marquette University; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; Fonds De La Recherche Scientifique - FNRS; Gordon and Betty Moore Foundation; Science Mission Directorate; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Fonds Wetenschappelijk Onderzoek","keywords":"Blazar; Neutrino; Flare; Neutrino astronomy; Coincidence; Neutrino detector; Flux (metallurgy); COSMIC cancer database","score_opus":0.005785446945849637,"score_gpt":0.1932369035425734,"score_spread":0.18745145659672374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913016105","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995928,0.00013015448,0.0006377887,0.00003557069,0.000014391004,0.000016394717,0.0014415262,0.000060056085,0.0017361398],"genre_scores_gemma":[0.9905461,0.000103951774,0.0023954874,0.000060461993,0.00003178924,0.000016087832,0.006182393,0.000038539005,0.0006252329],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965096,0.000035521414,0.000021905198,0.00010980984,0.00011179084,0.000070025744],"domain_scores_gemma":[0.99911934,0.000118398304,0.00033893404,0.00010970519,0.0001461547,0.00016747887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005553521,0.00031146244,0.00030158146,0.001707861,0.00045909165,0.0006701793,0.00033277684,0.00030260766,0.001199104],"category_scores_gemma":[0.0006505145,0.00017402352,0.0004035183,0.0011275869,0.00026991012,0.00017498342,0.0006285788,0.00027521272,0.0002829776],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057742064,0.00009681797,0.9544213,0.000049061684,0.0001587402,0.0017784366,0.00036298967,0.00059952616,0.031825688,0.00034163523,0.0010772233,0.008711204],"study_design_scores_gemma":[0.000014050432,0.000088534674,0.9897871,0.000012596827,0.000047934227,0.00097593764,0.00014406425,0.0012184299,0.0047170697,0.00006303931,0.0029214954,0.000009747488],"about_ca_topic_score_codex":0.006402526,"about_ca_topic_score_gemma":0.013934316,"teacher_disagreement_score":0.006402526,"about_ca_system_score_codex":0.0005575242,"about_ca_system_score_gemma":0.00033452694,"threshold_uncertainty_score":0.012730539},"labels":[],"label_agreement":null},{"id":"W2913094810","doi":"10.3847/1538-4357/ab0419","title":"The Next Generation Fornax Survey (NGFS). V. Discovery of a Dwarf–Dwarf Galaxy Pair at z = 0.30 and Its Characterization Using Deep VLT/MUSE Observations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Dwarf galaxy; Galaxy; Dwarf spheroidal galaxy; Astronomy; Dwarf galaxy problem; Local Group; Interacting galaxy","score_opus":0.0397406439336912,"score_gpt":0.2297362651547547,"score_spread":0.1899956212210635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913094810","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9770355,0.000524214,0.0003423777,0.000255635,0.000024635143,0.00005870965,0.012072056,0.00008046721,0.009606227],"genre_scores_gemma":[0.9707181,0.0002232765,0.002355695,0.00016987762,0.000035345605,0.00004861128,0.020596383,0.000014073703,0.005838681],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999851,0.000024741743,0.000009401792,0.000032921995,0.000044837325,0.00003714643],"domain_scores_gemma":[0.99965537,0.000019066347,0.00008345966,0.00003947054,0.000056094024,0.00014651497],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049326324,0.00014981069,0.00017888584,0.001151868,0.0003920571,0.000245351,0.00026862006,0.000162855,0.0021518387],"category_scores_gemma":[0.0004044674,0.00007298493,0.00012490453,0.0004556654,0.00011432792,0.00022261855,0.00062736624,0.00014333242,0.00047105513],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020575568,0.000045450914,0.9558151,0.000044039767,0.00005493213,0.00035874778,0.00041400365,0.00011730764,0.008779708,0.0006106746,0.0055580614,0.02799628],"study_design_scores_gemma":[0.0000113717,0.000053112406,0.99046665,0.0000122485735,0.000013760756,0.00021536656,0.0001344384,0.00019966724,0.00052022847,0.00013759529,0.008231767,0.0000036731076],"about_ca_topic_score_codex":0.025989035,"about_ca_topic_score_gemma":0.054462627,"teacher_disagreement_score":0.025989035,"about_ca_system_score_codex":0.00054734753,"about_ca_system_score_gemma":0.0003560893,"threshold_uncertainty_score":0.0516755},"labels":[],"label_agreement":null},{"id":"W2913202075","doi":"10.3847/1538-4357/ab01cc","title":"Radio Variability from a Quiescent Stellar-mass Black Hole Jet","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Black hole (networking); Flux (metallurgy); Accretion (finance); Active galactic nucleus; Jet (fluid); Sigma; Standard deviation; Binary number; Astronomy; Galaxy; Statistics","score_opus":0.009810890201755447,"score_gpt":0.21654573656036302,"score_spread":0.2067348463586076,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913202075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999206,0.000079277794,0.00017598965,0.0000142152285,0.0000026127648,0.0000015031602,0.000086660635,0.000010864201,0.0004228824],"genre_scores_gemma":[0.99958545,0.000028748464,0.00007251867,0.00001177208,0.000011939539,0.0000015959971,0.00019995622,0.0000021131027,0.0000859546],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999331,0.000008342264,0.0000047189787,0.000018333363,0.000018797753,0.000016573684],"domain_scores_gemma":[0.9995161,0.00009569006,0.0002278117,0.000044723805,0.000057655878,0.00005798109],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028517513,0.00011724579,0.00014539863,0.000556733,0.00018010732,0.00056397147,0.00020940835,0.00016943047,0.0005886562],"category_scores_gemma":[0.0007792732,0.000090300884,0.00013709896,0.00027133382,0.00024745808,0.00019175629,0.00026951358,0.00015966434,0.00012984622],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011147611,0.000016730053,0.9676425,0.000015944863,0.00004483993,0.0004315207,0.0002031693,0.0003461305,0.024142494,0.000107892614,0.00022927442,0.0067079924],"study_design_scores_gemma":[0.0000012731882,0.000018746692,0.999138,0.0000018579767,0.0000068844975,0.00015417367,0.000024028797,0.00015370666,0.0003280624,0.000023456263,0.00014811446,0.0000015747195],"about_ca_topic_score_codex":0.002074321,"about_ca_topic_score_gemma":0.0024620139,"teacher_disagreement_score":0.002074321,"about_ca_system_score_codex":0.00030130384,"about_ca_system_score_gemma":0.00004708533,"threshold_uncertainty_score":0.0041244626},"labels":[],"label_agreement":null},{"id":"W2913266227","doi":"10.3847/1538-4357/aaf857","title":"ALMA Observations of the ρ Ophiuchus B2 Region. I. Molecular Outflows and Their Driving Sources","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Ophiuchus; Protostar; Physics; Astrophysics; Outflow; Serpens; Basso continuo; Astronomy; Molecular cloud; Young stellar object; Submillimeter Array; Magnetic field; Star formation; Stars","score_opus":0.01194583410623917,"score_gpt":0.20802395125803666,"score_spread":0.1960781171517975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913266227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984225,0.000041455525,0.00015445621,0.000011437599,0.0000014337613,0.0000034175864,0.00021364754,0.000017890485,0.0011338448],"genre_scores_gemma":[0.9988728,0.000023631186,0.0003759506,0.000010576021,0.000006538368,0.0000043376963,0.0004476863,0.0000036689585,0.00025465738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999074,0.000008135542,0.0000035542503,0.000022528777,0.000029312641,0.000029050989],"domain_scores_gemma":[0.99985087,0.0000109610955,0.000032972046,0.00001487972,0.000027058588,0.000063170904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014043137,0.0001544962,0.00014077433,0.00084910006,0.0004329605,0.00041448345,0.00015088862,0.00014676887,0.0008669882],"category_scores_gemma":[0.00020508685,0.000114681134,0.00012615888,0.00040637917,0.0001279811,0.00018931318,0.00038362225,0.00015063763,0.00013729205],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071946246,0.00014025993,0.6546712,0.00005348092,0.000091311886,0.0005394828,0.0005497364,0.00081069494,0.32486033,0.00045325453,0.00086013693,0.016250674],"study_design_scores_gemma":[0.000021925971,0.0000636007,0.9920229,0.000005464081,0.000015959213,0.00014815459,0.00014392991,0.0010814755,0.0049317917,0.000066778186,0.0014920384,0.0000059241434],"about_ca_topic_score_codex":0.008379843,"about_ca_topic_score_gemma":0.013956695,"teacher_disagreement_score":0.008379843,"about_ca_system_score_codex":0.00035505812,"about_ca_system_score_gemma":0.00017728694,"threshold_uncertainty_score":0.01666212},"labels":[],"label_agreement":null},{"id":"W2913305412","doi":"10.3847/1538-4357/ab0081","title":"A New Generation of Cool White Dwarf Atmosphere Models. III. WD J2356–209: Accretion of a Planetesimal with an Unusual Composition","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planetesimal; White dwarf; Physics; Astrophysics; Photosphere; Atmosphere (unit); Accretion (finance); Astronomy; Spectral line; Planet; Stars","score_opus":0.01309502884042513,"score_gpt":0.21473786805933937,"score_spread":0.20164283921891424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913305412","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.72499275,0.0012716939,0.23402062,0.002401512,0.00038856865,0.00020372865,0.0025660738,0.0019111536,0.032243874],"genre_scores_gemma":[0.9349917,0.0005752293,0.05449128,0.00033527796,0.00033572316,0.00024964943,0.0014166606,0.00063916616,0.0069653676],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998698,0.000052576186,0.000006966439,0.00002082714,0.000022201351,0.000027642152],"domain_scores_gemma":[0.9995216,0.0001827171,0.000066624845,0.000051104336,0.00008187926,0.000096081065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004396304,0.00095414114,0.00096265133,0.00067500124,0.0008784371,0.0015118719,0.0018697976,0.0012987067,0.0023548857],"category_scores_gemma":[0.0015502098,0.00060424936,0.0016922043,0.00031828557,0.0005173437,0.00088991295,0.0013369031,0.0010428498,0.00038768433],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000115533585,0.00012683135,0.006631456,0.00006617367,0.00019644793,0.00023770495,0.0001043975,0.9695617,0.0023647475,0.012982373,0.0016037467,0.0060088765],"study_design_scores_gemma":[0.000052988442,0.000015604624,0.00047919073,0.0000044576996,0.000021935602,0.00001846064,0.0000127877265,0.99620336,0.000112121335,0.0022085733,0.0008607713,0.000009779541],"about_ca_topic_score_codex":0.015436231,"about_ca_topic_score_gemma":0.011368015,"teacher_disagreement_score":0.015436231,"about_ca_system_score_codex":0.0006732142,"about_ca_system_score_gemma":0.00074913044,"threshold_uncertainty_score":0.030692756},"labels":[],"label_agreement":null},{"id":"W2913804985","doi":"10.3847/1538-4357/aaf861","title":"Spitzer Microlensing of MOA-2016-BLG-231L: A Counter-rotating Brown Dwarf Binary in the Galactic Disk","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Gravitational microlensing; Physics; Brown dwarf; Astrophysics; Astronomy; Light curve; Proper motion; Circumbinary planet; Binary number; Caustic (mathematics); Mass ratio; Stars","score_opus":0.009148454457011073,"score_gpt":0.2260217355790405,"score_spread":0.21687328112202944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913804985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992017,0.000044751494,0.00008670267,0.000024017545,0.0000031973682,0.000002691304,0.00018921772,0.000012525523,0.00043525573],"genre_scores_gemma":[0.99923146,0.000011248525,0.00011920028,0.000007921651,0.0000061364694,0.0000011686196,0.0004860807,0.0000042794663,0.0001325047],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998604,0.000010829284,0.000006157067,0.000035067143,0.000037753565,0.000049662816],"domain_scores_gemma":[0.99958247,0.00004113462,0.0001328551,0.000028344624,0.00003589656,0.00017934063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020615419,0.00021368371,0.00034859544,0.0011027451,0.0005393349,0.0007083346,0.00022223066,0.00029422744,0.00066413364],"category_scores_gemma":[0.00041949874,0.00008931586,0.0002515043,0.00052132807,0.00031207147,0.00025571176,0.0006733512,0.00027893102,0.0002456335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049702765,0.00017100177,0.94180644,0.000038348484,0.00012534007,0.0034455361,0.00039681446,0.0015235874,0.04200139,0.0014412218,0.00090154965,0.0076517137],"study_design_scores_gemma":[0.000018493887,0.00007615518,0.9883394,0.000005508703,0.00002651149,0.00094992423,0.00025412746,0.005799532,0.0027099226,0.0003605351,0.0014450729,0.000014731049],"about_ca_topic_score_codex":0.0063719493,"about_ca_topic_score_gemma":0.008793764,"teacher_disagreement_score":0.0063719493,"about_ca_system_score_codex":0.00078687933,"about_ca_system_score_gemma":0.00019537623,"threshold_uncertainty_score":0.012669742},"labels":[],"label_agreement":null},{"id":"W2913874811","doi":"10.3847/1538-4357/aafad5","title":"Spectral Sequences of Type Ia Supernovae. II. Carbon as a Diagnostic Tool for Explosion Mechanisms","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Carbon fibers; Spectral line; Line (geometry); Range (aeronautics); Opacity; White dwarf","score_opus":0.01119220541067657,"score_gpt":0.24033453326051737,"score_spread":0.22914232784984082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2913874811","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99019974,0.00014107906,0.002556602,0.000022629874,0.0000075491753,0.000025401148,0.0019960096,0.00013306661,0.0049179816],"genre_scores_gemma":[0.99606043,0.000051390223,0.0015289033,0.0000066766374,0.0000042062748,0.000009869425,0.0017829575,0.000017175378,0.0005383092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999449,0.000008906505,0.0000064053206,0.000014652658,0.000012529437,0.000012611316],"domain_scores_gemma":[0.9993191,0.00016588521,0.00019830737,0.00005055206,0.00015151154,0.00011465161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022267099,0.00020921057,0.00010703116,0.0022383502,0.00019954276,0.00033826986,0.00014927752,0.00025645128,0.0023537884],"category_scores_gemma":[0.00084055687,0.00007892829,0.00024412014,0.0005911866,0.00015052363,0.00019637766,0.00019706678,0.0001271589,0.00048667623],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055926177,0.00009162453,0.9244803,0.00007056683,0.0000867568,0.00030033532,0.00015500892,0.009554796,0.037043616,0.0019780947,0.0008933053,0.024786174],"study_design_scores_gemma":[0.0000065615964,0.00007942255,0.98363125,0.000010332365,0.000019296387,0.00035317484,0.0000807618,0.009882487,0.004191356,0.00097432535,0.0007632484,0.000007814131],"about_ca_topic_score_codex":0.0016154104,"about_ca_topic_score_gemma":0.0018198894,"teacher_disagreement_score":0.0023537884,"about_ca_system_score_codex":0.00022712133,"about_ca_system_score_gemma":0.00007982404,"threshold_uncertainty_score":0.007874191},"labels":[],"label_agreement":null},{"id":"W2914173109","doi":"10.3847/1538-4357/ab0201","title":"The SAMI Galaxy Survey: Quenching of Star Formation in Clusters I. Transition Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Australian Astronomical Optics-Macquarie; Australian Research Council; Natural Sciences and Engineering Research Council of Canada","keywords":"Astrophysics; Physics; Velocity dispersion; Galaxy cluster; Galaxy; Star formation; Population; Galaxy group; Cluster (spacecraft); Astronomy; Brightest cluster galaxy","score_opus":0.007885826766394991,"score_gpt":0.2088655393420556,"score_spread":0.2009797125756606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2914173109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959189,0.0001346684,0.00016880686,0.000029921674,0.0000019272572,0.000008840764,0.0025460033,0.00005656026,0.0011344203],"genre_scores_gemma":[0.99706846,0.000051461568,0.00026112713,0.000009747531,0.000004864912,0.000005669971,0.0024455937,0.000006207287,0.00014687142],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982375,0.00003545052,0.000008260297,0.000051388964,0.000049575352,0.00003166245],"domain_scores_gemma":[0.99926347,0.00007953536,0.00030006285,0.00007668489,0.000106492924,0.00017371606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037370637,0.00015288565,0.00018911256,0.0016052786,0.00024672705,0.00032556648,0.0002940253,0.00015353326,0.0010872212],"category_scores_gemma":[0.0007928776,0.00009044049,0.0001709171,0.0013854338,0.00016033348,0.0002285847,0.00038597142,0.00016945825,0.00029764758],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037319005,0.000012157525,0.9948814,0.000008982857,0.000020401014,0.000012066332,0.000056515455,0.00019405034,0.0008902486,0.000061987856,0.0004633668,0.0033614296],"study_design_scores_gemma":[0.0000011473907,0.000008802222,0.99942267,0.0000010504716,0.0000029831124,0.000013665965,0.00002161147,0.00024890088,0.00009425271,0.000011062223,0.00017305333,8.250486e-7],"about_ca_topic_score_codex":0.015583369,"about_ca_topic_score_gemma":0.019777503,"teacher_disagreement_score":0.015583369,"about_ca_system_score_codex":0.000459485,"about_ca_system_score_gemma":0.00016579863,"threshold_uncertainty_score":0.030985296},"labels":[],"label_agreement":null},{"id":"W2914266888","doi":"10.3847/1538-4357/ab010a","title":"Detection of Nonthermal Hard X-Ray Emission from the “Fermi Bubble” in an External Galaxy","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Galaxy; Milky Way; Synchrotron radiation; Cosmic microwave background; Synchrotron; Spectral line; Electron; Compton scattering","score_opus":0.0077421726563676255,"score_gpt":0.21589275660776058,"score_spread":0.20815058395139296,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2914266888","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986739,0.000056836,0.0002073745,0.0000144159085,0.000003053261,0.000002310788,0.0000627013,0.00002301304,0.00095635746],"genre_scores_gemma":[0.99942565,0.000012370874,0.00022335666,0.000013089208,0.000003847009,0.0000017972131,0.00013669793,0.000004578887,0.00017866862],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999193,0.0000057147454,0.0000032077794,0.000021218886,0.000023290659,0.000027335433],"domain_scores_gemma":[0.99958116,0.00004980896,0.00010106155,0.000058394966,0.0000557935,0.00015380328],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001470569,0.00018266158,0.00021978944,0.0005137449,0.00026788452,0.00038158701,0.00023548851,0.00022844285,0.0015541486],"category_scores_gemma":[0.0002689894,0.0001293667,0.00015505435,0.00017286537,0.00039292945,0.00018033794,0.00053615577,0.00025222305,0.0002690145],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004822061,0.000107001375,0.728261,0.000093900264,0.0001136578,0.0028076987,0.0007263939,0.0002732506,0.25252768,0.0011508127,0.0010544666,0.012402023],"study_design_scores_gemma":[0.000015904954,0.00016554451,0.9803925,0.00001750004,0.000038082097,0.0017582739,0.0002601804,0.0010421874,0.013887686,0.00021964699,0.0021911985,0.000011335917],"about_ca_topic_score_codex":0.0025243054,"about_ca_topic_score_gemma":0.0029677446,"teacher_disagreement_score":0.0025243054,"about_ca_system_score_codex":0.00025558088,"about_ca_system_score_gemma":0.00010315444,"threshold_uncertainty_score":0.005199194},"labels":[],"label_agreement":null},{"id":"W2914842362","doi":"10.3847/1538-4357/ab4597","title":"Milky Way Halo Vibrations and Incommensurate Stream Velocities","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Dark matter; Halo; Galactic halo; Dark matter halo; Quadrupole; Gravitational potential","score_opus":0.009926155023819641,"score_gpt":0.24846213548097418,"score_spread":0.23853598045715455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2914842362","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989685,0.000019034904,0.0005079148,0.000012223092,0.0000012128091,0.0000013808444,0.000025540938,0.000012505474,0.00045164907],"genre_scores_gemma":[0.99955684,0.0000146840075,0.00014600148,0.0000020371301,9.589046e-7,0.0000015078236,0.00004126153,0.000005406423,0.00023126966],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999249,0.0000136533245,0.000004598552,0.000019646037,0.000016463495,0.000020661906],"domain_scores_gemma":[0.9994485,0.00015190635,0.00017211224,0.00005859159,0.00005697716,0.000111865884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025700277,0.00019495269,0.00016548733,0.0005642798,0.00022212473,0.0007697784,0.00022654429,0.0002340595,0.0013619006],"category_scores_gemma":[0.002716189,0.00017690143,0.00020713756,0.00033658167,0.0004272804,0.00052290724,0.0005179086,0.00022035262,0.00018251134],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005776572,0.00009069935,0.8036876,0.00005070809,0.00008916274,0.00061835395,0.0009272378,0.14042524,0.0271892,0.013865798,0.0004548343,0.0120236045],"study_design_scores_gemma":[0.00005817039,0.00013505998,0.5257519,0.000015028259,0.000038381313,0.00022775977,0.00045091187,0.45737997,0.0076291934,0.0074022715,0.00086481747,0.000046447636],"about_ca_topic_score_codex":0.003606647,"about_ca_topic_score_gemma":0.0021534949,"teacher_disagreement_score":0.003606647,"about_ca_system_score_codex":0.00047624274,"about_ca_system_score_gemma":0.00021744987,"threshold_uncertainty_score":0.007171333},"labels":[],"label_agreement":null},{"id":"W2914864461","doi":"10.3847/1538-4357/ab05c7","title":"The Mass Evolution of Protostellar Disks and Envelopes in the Perseus Molecular Cloud","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Canadian Space Agency; U.S. Department of Defense; European Commission; Academia Sinica; Koninklijke Nederlandse Akademie van Wetenschappen; National Science Foundation; Compute Canada; Canarie; Canadian Foundation for AIDS Research; Smithsonian Astrophysical Observatory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Smithsonian Institution","keywords":"Protostar; Physics; Astrophysics; Star formation; Molecular cloud; Astronomy; Mass distribution; Stars; Stellar evolution; Stellar mass; Galaxy","score_opus":0.004766837777301571,"score_gpt":0.21550243160814522,"score_spread":0.21073559383084364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2914864461","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995814,0.000045532997,0.000050357,0.0000042122924,3.4249405e-7,0.0000010374164,0.0000817749,0.0000027131634,0.00023256456],"genre_scores_gemma":[0.9997296,0.00001586597,0.000081802005,0.000002047959,6.587653e-7,5.932992e-7,0.00011418073,7.38106e-7,0.000054548713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999317,0.000008761502,0.0000036027704,0.000025071702,0.00001810667,0.000012729918],"domain_scores_gemma":[0.99971145,0.000052609084,0.00010902737,0.000029089399,0.00004243047,0.000055380682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013849899,0.00016452553,0.000093468916,0.0010567945,0.0002001949,0.00035432976,0.00023957195,0.0001128601,0.00042742424],"category_scores_gemma":[0.00071743777,0.00006981216,0.00007783926,0.00041213143,0.00019009947,0.0001876419,0.00033302914,0.00008097621,0.00012625901],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050609557,0.000011315546,0.98683214,0.000006315311,0.000020979387,0.00013499937,0.00020504654,0.0010664633,0.0067389216,0.0001708299,0.00006438068,0.0046980875],"study_design_scores_gemma":[0.000002033014,0.000015992571,0.99638677,0.0000024104656,0.0000034906864,0.00010056235,0.00013455036,0.0019107747,0.0011552786,0.000063449836,0.00022314477,0.000001504645],"about_ca_topic_score_codex":0.012798962,"about_ca_topic_score_gemma":0.0145870475,"teacher_disagreement_score":0.012798962,"about_ca_system_score_codex":0.00048020683,"about_ca_system_score_gemma":0.00010546346,"threshold_uncertainty_score":0.025448918},"labels":[],"label_agreement":null},{"id":"W2914875546","doi":"10.3847/1538-4357/ab0085","title":"Dancing in the Dark: Uncertainty in Ultrafaint Dwarf Galaxy Predictions from Cosmological Simulations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Dwarf galaxy; Reionization; Galaxy; Metallicity; Star formation; Dwarf galaxy problem; Stars; Halo; Galaxy formation and evolution; Astronomy; Stellar mass; Local Group; Interacting galaxy; Redshift","score_opus":0.009842567819875421,"score_gpt":0.22540416598912716,"score_spread":0.21556159816925174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2914875546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906013,0.00018255964,0.006116808,0.00047502757,0.000019105639,0.000010460114,0.00047298975,0.00018216936,0.0019394465],"genre_scores_gemma":[0.99847084,0.00003659895,0.0010973609,0.0000615607,0.000008309736,0.000005320909,0.00020052053,0.000033947545,0.00008540771],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987931,0.0006514874,0.000060363476,0.00022474212,0.00016127888,0.00010890395],"domain_scores_gemma":[0.9766688,0.017608123,0.0014763994,0.0022643618,0.0009135361,0.0010688008],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0051994086,0.000490299,0.0006030546,0.00077452697,0.0007923337,0.0015548125,0.0016365569,0.00085227063,0.0010183618],"category_scores_gemma":[0.034575336,0.0004614429,0.00044511788,0.0006763087,0.0010646593,0.0016483229,0.0010553503,0.0010038351,0.0001420426],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022789254,0.000064786545,0.10218542,0.00004648451,0.00017109058,0.00011025882,0.00022708334,0.8868897,0.00063202507,0.00491657,0.0007257535,0.0038028816],"study_design_scores_gemma":[0.000035061374,0.00003111905,0.012977004,0.000019349456,0.000021021131,0.0000180162,0.00008605826,0.97811127,0.00047677284,0.007896939,0.00030285286,0.000024573616],"about_ca_topic_score_codex":0.034269635,"about_ca_topic_score_gemma":0.019441446,"teacher_disagreement_score":0.034269635,"about_ca_system_score_codex":0.001243737,"about_ca_system_score_gemma":0.0007435966,"threshold_uncertainty_score":0.06814033},"labels":[],"label_agreement":null},{"id":"W2914946979","doi":"10.3847/1538-4357/ab0086","title":"Magnetic Field Structure of Dense Cores Using Spectroscopic Methods","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Magnetic field; Field strength; Field (mathematics); Context (archaeology); Polarization (electrochemistry); Computational physics; Magnetic flux; Dispersion (optics); Physics; Flux (metallurgy); Kinematics; Astrophysics; Materials science; Geology; Optics; Chemistry; Classical mechanics","score_opus":0.011240819659299815,"score_gpt":0.2972240080694769,"score_spread":0.2859831884101771,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2914946979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92985314,0.00010992317,0.06634992,0.00007658776,0.0000065460235,0.000036637262,0.00023924516,0.00022707097,0.0031008373],"genre_scores_gemma":[0.9961987,0.000020105797,0.0035017463,0.0000059045747,0.00000505008,0.000007484211,0.00007749676,0.0000049152072,0.00017858071],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999633,0.000008941732,0.000001317098,0.000009930384,0.000010427717,0.000006123127],"domain_scores_gemma":[0.9998203,0.00003980136,0.000060531675,0.00002382348,0.000031145726,0.000024436025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019088596,0.0002829174,0.00014560118,0.0005971324,0.00019211555,0.00030601252,0.0004042024,0.00023143429,0.00046222142],"category_scores_gemma":[0.0007775601,0.00019627377,0.00018484889,0.00021679587,0.00025599496,0.00037232006,0.000243382,0.00014786667,0.00010283231],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001257237,0.00009298361,0.15121461,0.000029672336,0.00005803404,0.00018879268,0.00009759432,0.7852201,0.03551839,0.008788408,0.0004954011,0.018170346],"study_design_scores_gemma":[0.000013771611,0.000012216025,0.017857255,0.000002794358,0.0000025563675,0.000014594059,0.000009338702,0.97873676,0.0009856028,0.002223237,0.000136443,0.000005381598],"about_ca_topic_score_codex":0.010572653,"about_ca_topic_score_gemma":0.0071572466,"teacher_disagreement_score":0.010572653,"about_ca_system_score_codex":0.00051155966,"about_ca_system_score_gemma":0.00032310886,"threshold_uncertainty_score":0.0210222},"labels":[],"label_agreement":null},{"id":"W2915081011","doi":"10.3847/1538-4357/ab0ae9","title":"Dust Continuum Emission and the Upper Limit Fluxes of Submillimeter Water Lines of the Protoplanetary Disk around HD 163296 Observed by ALMA","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Korea Astronomy and Space Science Institute; Yukawa Institute for Theoretical Physics, Kyoto University; European Southern Observatory; National Astronomical Observatory of Japan; Queen's University; National Science Council; Japan Society for the Promotion of Science; Queen's University Belfast; Academia Sinica; University of Leeds; National Radio Astronomy Observatory; National Science Foundation","keywords":"Opacity; Millimeter; Submillimeter Array; Protoplanetary disk; Planet; Position angle; Cosmic dust; Snow line","score_opus":0.009418619244285859,"score_gpt":0.20133596939164097,"score_spread":0.19191735014735511,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2915081011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99912983,0.000068815236,0.00024015098,0.000008121779,0.0000011422525,9.92301e-7,0.00006976034,0.000015572108,0.0004656305],"genre_scores_gemma":[0.99964535,0.000018035573,0.00016019808,0.000005342569,0.0000024811607,0.0000013135915,0.000101698046,0.0000031663667,0.000062302504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999566,0.0000042522,0.000002027214,0.00001476374,0.000011322948,0.000011025066],"domain_scores_gemma":[0.9998117,0.00004875867,0.00007562622,0.000016217178,0.000017659995,0.000029964525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000122029174,0.00018130415,0.00019234502,0.00045389647,0.00022099183,0.00030763337,0.00019450039,0.00023392006,0.00089935947],"category_scores_gemma":[0.00026254504,0.00013004807,0.00018647987,0.00020490722,0.0001281666,0.00028602744,0.00019701569,0.00017171279,0.00018494885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030593676,0.00007625914,0.86711776,0.000049242044,0.000089281886,0.00061883405,0.0002728024,0.0025855312,0.11849908,0.00024593752,0.00026780722,0.009871617],"study_design_scores_gemma":[0.000009186625,0.000022880115,0.9929196,0.0000035788162,0.000012729237,0.00007757313,0.00006171848,0.0031141161,0.0033687558,0.00007928165,0.00032718552,0.0000033897122],"about_ca_topic_score_codex":0.0018880697,"about_ca_topic_score_gemma":0.0029975732,"teacher_disagreement_score":0.0018880697,"about_ca_system_score_codex":0.0002146287,"about_ca_system_score_gemma":0.000038424216,"threshold_uncertainty_score":0.0037541986},"labels":[],"label_agreement":null},{"id":"W2915258689","doi":"10.3847/1538-4357/ab002a","title":"Confirming Herschel Candidate Protoclusters from ALMA/VLA CO Observations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Astronomical Observatory of Japan; National Research Foundation; National Institutes of Natural Sciences; Danmarks Grundforskningsfond; National Radio Astronomy Observatory; Villum Fonden; Korea Astronomy and Space Science Institute; Ministerio de Economía y Competitividad; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Star formation; Astronomy; Population","score_opus":0.013316345815686555,"score_gpt":0.23250693681001008,"score_spread":0.21919059099432353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2915258689","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950578,0.00028403354,0.0010978706,0.000058631635,0.0000121432595,0.00001878795,0.000421068,0.000119574885,0.0029301383],"genre_scores_gemma":[0.99700963,0.00005215476,0.0016134243,0.000067282286,0.000011994999,0.0000070249225,0.0006438641,0.000009953122,0.0005846571],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973375,0.00001105456,0.00000774344,0.00007893481,0.00009910515,0.000069346934],"domain_scores_gemma":[0.9992093,0.00007023324,0.00023498072,0.00009346058,0.00014568109,0.00024634082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003021997,0.00022400741,0.00017014003,0.0011313899,0.00050464395,0.0007504398,0.00051917275,0.00038957674,0.0017040304],"category_scores_gemma":[0.00063311215,0.0001436663,0.00015392098,0.0003765411,0.00031176786,0.00033408232,0.00080890715,0.00024869107,0.0007141631],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013730084,0.000062586885,0.8317893,0.00003864108,0.00004474653,0.0008999139,0.00034900222,0.00023265228,0.1502167,0.0005265413,0.0010397816,0.014662705],"study_design_scores_gemma":[0.00001641063,0.000108203,0.9569523,0.000016780838,0.000026662548,0.0011143514,0.0003606051,0.0026259974,0.032737885,0.0002714993,0.005752669,0.000016623468],"about_ca_topic_score_codex":0.003927854,"about_ca_topic_score_gemma":0.008235431,"teacher_disagreement_score":0.003927854,"about_ca_system_score_codex":0.00050116924,"about_ca_system_score_gemma":0.0001847821,"threshold_uncertainty_score":0.0078099966},"labels":[],"label_agreement":null},{"id":"W2915381923","doi":"10.3847/1538-4357/aba521","title":"Limits on Protoplanet Growth by Accretion of Small Solids","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Pebble; Sublimation (psychology); Physics; Astrophysics; Debris; Turbulence; RADIUS; Accretion (finance); Opacity; Mechanics; Meteorology; Geology; Geomorphology","score_opus":0.01490236418145768,"score_gpt":0.20709592959011766,"score_spread":0.19219356540865998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2915381923","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98191535,0.0004837342,0.008795815,0.00021231992,0.000008554697,0.0000055141227,0.00020895446,0.00010733746,0.008262347],"genre_scores_gemma":[0.9989862,0.00011688054,0.00054694805,0.000012196713,0.000004184535,0.000004084164,0.00010112226,0.000015769005,0.00021252171],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999848,0.00002607692,0.0000075848934,0.000036498677,0.000037033697,0.000044735367],"domain_scores_gemma":[0.9974764,0.0015898967,0.00030804233,0.00024087608,0.00014891336,0.00023580928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038811847,0.0004997027,0.0005847767,0.0004568508,0.0005527565,0.0013202211,0.00076078693,0.00056253746,0.0019202058],"category_scores_gemma":[0.0036184604,0.0002744709,0.00053622684,0.00019617965,0.0008086825,0.00091764174,0.0008942543,0.00045885844,0.00031702485],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069589354,0.00008491223,0.06141809,0.00018343805,0.00008019694,0.0004805644,0.00028142662,0.8388602,0.044031467,0.042012822,0.0009109769,0.010960102],"study_design_scores_gemma":[0.000059263766,0.00017410502,0.021365408,0.000044043274,0.000040219824,0.0002582371,0.00013999568,0.9369942,0.014707761,0.023539925,0.0026296987,0.00004719047],"about_ca_topic_score_codex":0.009651192,"about_ca_topic_score_gemma":0.0035442123,"teacher_disagreement_score":0.009651192,"about_ca_system_score_codex":0.001164194,"about_ca_system_score_gemma":0.0003993579,"threshold_uncertainty_score":0.019190013},"labels":[],"label_agreement":null},{"id":"W2915654042","doi":"10.3847/1538-4357/ab0958","title":"The JCMT BISTRO Survey: The Magnetic Field in the Starless Core <i>ρ</i> Ophiuchus C","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Dalhousie University; Western University; University of Manitoba; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"Japan Society for the Promotion of Science; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; East Asian Core Observatories Association; National Astronomical Observatory of Japan; National Research Foundation of Korea; China Scholarship Council; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; Chinese Academy of Sciences; Academia Sinica; National Natural Science Foundation of China; Science and Technology Facilities Council; National Research Foundation; Chinese University of Hong Kong; Ministry of Science, ICT and Future Planning; Ministry of Science and Technology, Taiwan; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Smithsonian Institution","keywords":"Ophiuchus; James Clerk Maxwell Telescope; Physics; Astrophysics; Magnetic field; Sky; Molecular cloud; Polarization (electrochemistry); Star formation; Stars; Chemistry","score_opus":0.014365493320145301,"score_gpt":0.2453986296526285,"score_spread":0.2310331363324832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2915654042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99795425,0.00005370395,0.00012775876,0.00002500819,0.0000020219027,0.000008649938,0.00082202663,0.000031453415,0.00097500556],"genre_scores_gemma":[0.99714464,0.00006232233,0.00053195166,0.0000337679,0.000015419593,0.000007747789,0.0019553176,0.000011490418,0.0002373589],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984777,0.000010850464,0.000008119324,0.000034752426,0.000057207024,0.000041290466],"domain_scores_gemma":[0.9992513,0.000040487368,0.00026962342,0.00007357581,0.00013179012,0.0002332346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018521534,0.00021983492,0.00018186808,0.0017020062,0.0005024938,0.00035758628,0.00033356168,0.00020077125,0.00060936593],"category_scores_gemma":[0.0006193066,0.00011828961,0.00012788107,0.00096993346,0.00025196178,0.0002513909,0.0006318601,0.00018582011,0.00017366382],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015678363,0.000051803225,0.9552238,0.000032552023,0.00004729728,0.00029139107,0.0003829838,0.0002806568,0.030977424,0.0001534365,0.0009776844,0.011424187],"study_design_scores_gemma":[0.000004501987,0.000011949716,0.998216,0.0000023334849,0.0000058768965,0.00007197041,0.000039218732,0.00030266188,0.0007805436,0.000012585212,0.00055035757,0.0000018752529],"about_ca_topic_score_codex":0.029346203,"about_ca_topic_score_gemma":0.047732048,"teacher_disagreement_score":0.029346203,"about_ca_system_score_codex":0.0005612615,"about_ca_system_score_gemma":0.00035447776,"threshold_uncertainty_score":0.058350742},"labels":[],"label_agreement":null},{"id":"W2915692329","doi":"10.3847/1538-4357/ab089c","title":"A MegaCam Survey of Outer Halo Satellites. VII. A Single Sérsic Index versus Effective Radius Relation for Milky Way Outer Halo Satellites*†","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Halo; Surface brightness; RADIUS; Local Group; Dark matter halo; Galaxy; Globular cluster","score_opus":0.01307208906843102,"score_gpt":0.22584042480201003,"score_spread":0.212768335733579,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2915692329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99870133,0.00013076811,0.000095872834,0.000009502642,7.174718e-7,0.000001934294,0.00059353403,0.000007670546,0.0004585682],"genre_scores_gemma":[0.9974483,0.00006591969,0.00036170645,0.0000091950105,0.0000028911675,0.000003492526,0.0017585944,0.0000047690482,0.00034516872],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998779,0.000017246202,0.000009079968,0.00003572566,0.000032443946,0.00002754443],"domain_scores_gemma":[0.9992065,0.00007224898,0.00029705194,0.00013047626,0.00012246409,0.00017134122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003404735,0.00015195041,0.00015494706,0.0014342716,0.00013136871,0.00034454477,0.00020508704,0.00012294814,0.0006122654],"category_scores_gemma":[0.0005931135,0.00011724176,0.00019992577,0.0010382512,0.00012508487,0.0002582269,0.00069971214,0.000092026625,0.00021044015],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005042786,0.000008774104,0.98899406,0.000020937987,0.00005842637,0.000047122114,0.00022988216,0.000115981486,0.0029028214,0.00013380856,0.00023057337,0.0072071156],"study_design_scores_gemma":[0.0000013445843,0.0000069451808,0.9990343,0.0000023111324,0.00000795931,0.000030027355,0.00005180173,0.0001013955,0.00024993235,0.000013051693,0.000500069,9.092145e-7],"about_ca_topic_score_codex":0.00837452,"about_ca_topic_score_gemma":0.018438876,"teacher_disagreement_score":0.00837452,"about_ca_system_score_codex":0.00024906694,"about_ca_system_score_gemma":0.00015974231,"threshold_uncertainty_score":0.016651511},"labels":[],"label_agreement":null},{"id":"W2916025790","doi":"10.3847/1538-4357/ab0b41","title":"Size Scaling of Clump Instabilities in Turbulent, Feedback-regulated Disks","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Saint Mary's University","funders":"","keywords":"Galaxy; Scaling; Milky Way; Context (archaeology); Dynamo; Turbulence; Red clump; Instability; Galactic Center","score_opus":0.007620266959520545,"score_gpt":0.22623906176804945,"score_spread":0.21861879480852892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2916025790","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988373,0.000027692275,0.00089665875,0.000014901667,0.0000018322764,0.0000025015893,0.000022952752,0.00002137052,0.0001748579],"genre_scores_gemma":[0.9997454,0.000006948925,0.00019925206,0.000002152467,9.1213536e-7,0.0000018560346,0.000014284018,0.0000029350172,0.000026132819],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999368,0.000012994151,0.000004980642,0.000016775764,0.000012838956,0.00001549309],"domain_scores_gemma":[0.9993086,0.00027629102,0.00019084444,0.00007341076,0.00006544362,0.0000854581],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023956988,0.00022507294,0.00018716906,0.00039611085,0.00021622158,0.0005961356,0.00045061015,0.00028533288,0.00041798345],"category_scores_gemma":[0.0019950857,0.00014400753,0.00031076453,0.00015201156,0.0004230562,0.0003898054,0.00035697457,0.00025130511,0.000046842502],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005579211,0.00026891156,0.23594926,0.00008367188,0.0001764068,0.0005079683,0.00037969672,0.6508028,0.095438756,0.006387707,0.0003766264,0.009070255],"study_design_scores_gemma":[0.000045576093,0.00013228337,0.057981104,0.000007128497,0.00002096871,0.00006319869,0.000063152605,0.93096614,0.009098769,0.0014698517,0.0001314233,0.00002039261],"about_ca_topic_score_codex":0.003120127,"about_ca_topic_score_gemma":0.001495698,"teacher_disagreement_score":0.003120127,"about_ca_system_score_codex":0.0005737965,"about_ca_system_score_gemma":0.00018297326,"threshold_uncertainty_score":0.0062039495},"labels":[],"label_agreement":null},{"id":"W2917274298","doi":"10.3847/1538-4357/ab0966","title":"High-precision X-Ray Timing of Three Millisecond Pulsars with NICER: Stability Estimates and Comparison with Radio","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of British Columbia; McGill University","funders":"National Aeronautics and Space Administration","keywords":"Millisecond pulsar; Pulsar; Millisecond; Static timing analysis; Stability (learning theory); Pulse (music); Dispersion (optics); Residual; Scattering","score_opus":0.015817630931037014,"score_gpt":0.28947449654526,"score_spread":0.273656865614223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2917274298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99056834,0.00022539626,0.0063208914,0.000060387225,0.000011396536,0.000016560465,0.00079243374,0.00028996926,0.0017146418],"genre_scores_gemma":[0.99272776,0.000050464,0.004652763,0.000021413334,0.000028086535,0.0000107531805,0.002240354,0.000094495015,0.00017401224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992035,0.00009751636,0.00006482078,0.00020961954,0.0003322483,0.0000923438],"domain_scores_gemma":[0.9964155,0.0006239753,0.0013208084,0.00075247313,0.00063407054,0.0002531723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022784784,0.0002712451,0.00046042286,0.0021374312,0.00040216153,0.00086929946,0.0005827495,0.00033132854,0.0005051996],"category_scores_gemma":[0.004302794,0.00024260496,0.00049849454,0.0012252015,0.00036491465,0.00047671626,0.0009636296,0.00042064837,0.00029230688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012296448,0.00011115903,0.8034696,0.0001443759,0.00044433054,0.000389061,0.0007563349,0.019961854,0.122142926,0.0009827444,0.0007448047,0.04962327],"study_design_scores_gemma":[0.000034518704,0.00023889403,0.9657073,0.000013787262,0.00009857528,0.000416195,0.00007147824,0.02166491,0.00961347,0.00019597042,0.0019016954,0.000043210268],"about_ca_topic_score_codex":0.002314047,"about_ca_topic_score_gemma":0.003637877,"teacher_disagreement_score":0.002314047,"about_ca_system_score_codex":0.000435056,"about_ca_system_score_gemma":0.0001563861,"threshold_uncertainty_score":0.012049854},"labels":[],"label_agreement":null},{"id":"W2917786144","doi":"10.3847/1538-4357/ab3792","title":"The Brightest z ≳ 8 Galaxies over the COSMOS UltraVISTA Field","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Physics; Astronomy; Galaxy; Astrophysics; Cosmos (plant); Art history","score_opus":0.004381360338623136,"score_gpt":0.2028683594010415,"score_spread":0.19848699906241837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2917786144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984875,0.00007282621,0.00011147305,0.0000103393995,0.0000016882115,0.0000043083687,0.00021749025,0.000019713574,0.0010745729],"genre_scores_gemma":[0.99793017,0.000055632278,0.00025413334,0.000012326779,0.000007917312,0.0000077454515,0.00083282066,0.0000039174856,0.00089531444],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999874,0.000011561681,0.000005531728,0.000028045135,0.00003268275,0.00004821729],"domain_scores_gemma":[0.99955434,0.000038925664,0.00014620076,0.000040567797,0.000051969757,0.0001680472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015157879,0.00023073649,0.00021731101,0.0018915073,0.0003501035,0.000530092,0.0003531205,0.00012092434,0.004610452],"category_scores_gemma":[0.00032979724,0.00012962094,0.00014959628,0.00064851105,0.00019210602,0.0002943666,0.0006069147,0.000109722234,0.0009064608],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024782354,0.000055055483,0.96453977,0.000019584264,0.000026689951,0.00019934995,0.0002738501,0.00010097304,0.010487417,0.0002711252,0.0006232987,0.023155013],"study_design_scores_gemma":[0.000010037366,0.0000606804,0.9956898,0.000008329074,0.000014433078,0.0003523617,0.00018618151,0.00021394178,0.0010409353,0.000077567835,0.0023421247,0.000003590468],"about_ca_topic_score_codex":0.001995078,"about_ca_topic_score_gemma":0.0040115714,"teacher_disagreement_score":0.004610452,"about_ca_system_score_codex":0.00015417303,"about_ca_system_score_gemma":0.00009882849,"threshold_uncertainty_score":0.015423477},"labels":[],"label_agreement":null},{"id":"W2918104042","doi":"10.3847/1538-4357/ab2cd5","title":"SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z ∼ 6–7: Strong Associations of Dusty Star-forming Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Japan Society for the Promotion of Science; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; Ministério da Ciência, Tecnologia e Inovação; Ministerio de Ciencia, Tecnología e Innovación Productiva; Japan Science and Technology Agency; Cabinet Office, Government of Japan; Academia Sinica; Science and Technology Facilities Council; National Research Foundation; National Research Foundation of Korea; Princeton University; Ministry of Education, Culture, Sports, Science and Technology; Toray Science Foundation; National Science Foundation","keywords":"Galaxy; Redshift; Luminosity; Halo; Stars; Universe; Galaxy cluster; Luminous infrared galaxy; Star formation","score_opus":0.0073844688185918505,"score_gpt":0.2298107233616269,"score_spread":0.22242625454303505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2918104042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996391,0.00011543079,0.00030048797,0.00006973078,0.0000054622315,0.000003997481,0.00077255856,0.00004248264,0.0022988403],"genre_scores_gemma":[0.9971234,0.000040940668,0.0004618753,0.000019132152,0.000008372835,0.0000015600554,0.00091868406,0.000008403689,0.0014176891],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994874,0.0000038513435,0.000003130054,0.0000109790335,0.000018654036,0.000014767511],"domain_scores_gemma":[0.9996697,0.000034626057,0.000109329965,0.000040351257,0.000052193314,0.00009387068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013786704,0.000073020434,0.000074206466,0.0007799036,0.00019960101,0.00029336725,0.000097341726,0.00006836123,0.0024207986],"category_scores_gemma":[0.00030292748,0.000054361535,0.000100341,0.00030651092,0.00014584241,0.00014960769,0.0003148084,0.0001054881,0.0005861329],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009223358,0.00001884358,0.9668036,0.0000114590375,0.000017466515,0.00018455277,0.00024636445,0.00008038851,0.013417834,0.00019392958,0.0009439154,0.017989276],"study_design_scores_gemma":[7.255784e-7,0.000008702919,0.9981646,0.0000011988725,0.0000016479923,0.00005681054,0.000034070123,0.00006337547,0.0008036712,0.000024519086,0.0008400864,6.534352e-7],"about_ca_topic_score_codex":0.0036518187,"about_ca_topic_score_gemma":0.008304222,"teacher_disagreement_score":0.0036518187,"about_ca_system_score_codex":0.00015687403,"about_ca_system_score_gemma":0.0000648706,"threshold_uncertainty_score":0.0080984235},"labels":[],"label_agreement":null},{"id":"W2918121884","doi":"10.3847/1538-4357/ab0e15","title":"Search for Transient Gravitational-wave Signals Associated with Magnetar Bursts during Advanced LIGO’s Second Observing Run","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; Abdus Salam International Centre for Theoretical Physics; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Engineering and Physical Sciences Research Council; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; National Natural Science Foundation of China; European Commission; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; Conseil Régional, Île-de-France; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Engineering Research Board; National Science Foundation","keywords":"LIGO; Physics; Magnetar; Gravitational wave; Transient (computer programming); Astrophysics; Astronomy; Neutron star","score_opus":0.015585527851802929,"score_gpt":0.282142961878372,"score_spread":0.26655743402656906,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2918121884","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984211,0.000046172918,0.0005091507,0.000047318936,0.000005823223,0.0000084415915,0.00025070872,0.000041714393,0.0006696337],"genre_scores_gemma":[0.99754494,0.000015267222,0.00086519535,0.000029311877,0.00001649416,0.000013020732,0.0011574293,0.000011268419,0.0003470487],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993155,0.000096075346,0.000028704899,0.00015610163,0.00020993974,0.00019376556],"domain_scores_gemma":[0.99709976,0.0004475388,0.0006948153,0.00029987463,0.00026768513,0.0011903922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014354932,0.00066881423,0.0006984064,0.0018033432,0.0007895698,0.0010779724,0.00060451776,0.00077338866,0.0012714772],"category_scores_gemma":[0.001502292,0.00033380216,0.00063008186,0.00089359167,0.00043798587,0.00035944505,0.0015510574,0.0006430369,0.00028480997],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004795606,0.0006303498,0.8515536,0.00008967072,0.0004346119,0.0010094723,0.0009050478,0.0028457756,0.11690748,0.00067491323,0.0010988433,0.019054448],"study_design_scores_gemma":[0.00013668336,0.0011977433,0.9849518,0.000009885157,0.00010270975,0.00024006574,0.00017221214,0.0024708982,0.008782601,0.0001742363,0.0017209852,0.000040241863],"about_ca_topic_score_codex":0.0022092136,"about_ca_topic_score_gemma":0.004996843,"teacher_disagreement_score":0.0022092136,"about_ca_system_score_codex":0.0005899646,"about_ca_system_score_gemma":0.00039745533,"threshold_uncertainty_score":0.007591665},"labels":[],"label_agreement":null},{"id":"W2918921386","doi":"10.3847/1538-4357/ab0d80","title":"ALMA Observations of Layered Structures due to CO Selective Dissociation in the ρ Ophiuchi A Plane-parallel PDR","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Isotopologue; Dissociation (chemistry); Photodissociation; Astrochemistry; Interstellar medium; Molecular cloud; Angular diameter; Emission spectrum","score_opus":0.015043616267904543,"score_gpt":0.24526821735560667,"score_spread":0.23022460108770212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2918921386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984011,0.00006106456,0.0002561597,0.0000130592025,0.000001158953,0.000003768547,0.00020627456,0.00003243015,0.0010250169],"genre_scores_gemma":[0.9992065,0.00002827145,0.0003564372,0.000007777297,0.000003227594,0.000005075593,0.00022908012,0.000004894762,0.0001588239],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999392,0.0000051327524,0.0000021081291,0.000015391437,0.000021575675,0.000016578779],"domain_scores_gemma":[0.99987245,0.000014650967,0.000043907676,0.000012701188,0.00002508825,0.00003130999],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000079220044,0.00019754653,0.00015588898,0.0010762869,0.0002990359,0.00039681382,0.00021358207,0.00016200518,0.0007757705],"category_scores_gemma":[0.00020709512,0.00021049053,0.00017111914,0.0004989785,0.00020965807,0.00019090688,0.00042940347,0.00021339867,0.00018769647],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046247264,0.000055068904,0.33245686,0.000056292844,0.00014646593,0.00080754445,0.00044614135,0.000994528,0.6528442,0.00027438384,0.00036784555,0.011088177],"study_design_scores_gemma":[0.0000127617495,0.000042646203,0.98637056,0.0000049530763,0.000029611012,0.00030007798,0.00014216785,0.001653647,0.010428973,0.000053410848,0.00095437095,0.000006896013],"about_ca_topic_score_codex":0.0048981654,"about_ca_topic_score_gemma":0.0050870865,"teacher_disagreement_score":0.0048981654,"about_ca_system_score_codex":0.0002947002,"about_ca_system_score_gemma":0.00010379966,"threshold_uncertainty_score":0.00973928},"labels":[],"label_agreement":null},{"id":"W2920014427","doi":"10.3847/1538-4357/ab0c02","title":"The R-Process Alliance: Discovery of a Low-α, r-process-enhanced Metal-poor Star in the Galactic Halo","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Galaxy; Stars; Halo; Galactic halo; Dwarf galaxy; Galactic corona; Galactic tide; Stellar kinematics","score_opus":0.008197651368274954,"score_gpt":0.24439146848349025,"score_spread":0.23619381711521528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2920014427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99837446,0.00015644784,0.00014040704,0.00004712367,0.0000047285394,0.0000091062175,0.00013662527,0.000019639796,0.0011113684],"genre_scores_gemma":[0.99871254,0.00005187872,0.00031438755,0.00006122953,0.000008818073,0.0000028855598,0.00031678288,0.000008081831,0.0005235429],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998419,0.000010624878,0.000008141809,0.000042029424,0.000052511234,0.000044720633],"domain_scores_gemma":[0.9994542,0.000018695466,0.0000835228,0.000051041272,0.00006816295,0.0003243665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004927985,0.0003388284,0.00029072742,0.00090109295,0.00072620343,0.0007828007,0.00039365777,0.00028172636,0.0008833514],"category_scores_gemma":[0.00030947576,0.0001801027,0.00030633213,0.00049924804,0.00042437477,0.0002524078,0.0011249792,0.00031895598,0.00045621174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033883005,0.000118095646,0.884107,0.0000573607,0.00012995639,0.0041940818,0.0007753623,0.00015221695,0.09668546,0.0007093241,0.0010358746,0.011696289],"study_design_scores_gemma":[0.00002428553,0.00036520703,0.986355,0.0000109178745,0.000050605595,0.002803731,0.00045169407,0.0003358383,0.0040648417,0.0002186538,0.0053079776,0.000011156721],"about_ca_topic_score_codex":0.0045595104,"about_ca_topic_score_gemma":0.008284465,"teacher_disagreement_score":0.0045595104,"about_ca_system_score_codex":0.00044553322,"about_ca_system_score_gemma":0.00030100238,"threshold_uncertainty_score":0.009065926},"labels":[],"label_agreement":null},{"id":"W2921080121","doi":"10.3847/1538-4357/ab0ec1","title":"Gemini Imaging of the Host Galaxies of Changing-look Quasars","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Astrophysics; Physics; Quasar; Galaxy; Astronomy; Surface brightness; Active galactic nucleus; OVV quasar; Luminous infrared galaxy; Peculiar galaxy; Radio galaxy; Galaxy group","score_opus":0.004945013741598582,"score_gpt":0.20065075995331008,"score_spread":0.1957057462117115,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2921080121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973628,0.000049394876,0.00047734083,0.000028015385,0.0000026743878,0.00000513211,0.0005594366,0.00009353177,0.0014216917],"genre_scores_gemma":[0.99738103,0.000025503512,0.0013842785,0.000016158492,0.000005467174,0.0000023769155,0.0008267075,0.000013260836,0.00034520685],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999101,0.000006606647,0.0000030731587,0.000030660816,0.000021345299,0.000028192246],"domain_scores_gemma":[0.9997608,0.000019732806,0.000070166476,0.000026816377,0.000048582457,0.00007383748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023365901,0.00017982985,0.00011903471,0.0012733351,0.00025324133,0.00035150597,0.00020453343,0.00018494744,0.0009355226],"category_scores_gemma":[0.00023836279,0.00015741735,0.00012044032,0.0005913574,0.00009938807,0.00020941134,0.0002973665,0.00017654033,0.00018989386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003283765,0.000072954084,0.7943494,0.000036493864,0.000073812356,0.00036385912,0.0006761924,0.00086858735,0.18248484,0.000462063,0.0016100329,0.018673386],"study_design_scores_gemma":[0.0000043516047,0.000024604242,0.9927301,0.0000020325695,0.000016551541,0.000114401526,0.0001014879,0.0017168218,0.00432093,0.000033733795,0.0009311602,0.0000037564655],"about_ca_topic_score_codex":0.00478376,"about_ca_topic_score_gemma":0.0097484,"teacher_disagreement_score":0.00478376,"about_ca_system_score_codex":0.0003007723,"about_ca_system_score_gemma":0.00005587453,"threshold_uncertainty_score":0.009511828},"labels":[],"label_agreement":null},{"id":"W2921525166","doi":"10.3847/1538-4357/ab2da2","title":"On the Assembly Bias of Cool Core Clusters Traced by Hα Nebulae","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Halo; Cluster (spacecraft); Redshift; Sky; Galaxy cluster; Cluster analysis; Galaxy","score_opus":0.013116310499732074,"score_gpt":0.2187550878641079,"score_spread":0.20563877736437583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2921525166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99972147,0.00001681732,0.00012727952,0.0000030258661,3.901699e-7,5.436442e-7,0.00003176082,0.0000037672276,0.000094935844],"genre_scores_gemma":[0.999803,0.000005966233,0.00006605672,0.0000021353485,9.916022e-7,5.265667e-7,0.00009168268,0.0000023907792,0.00002737373],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976534,0.00004662376,0.000011109751,0.000093045026,0.000043730437,0.000040175026],"domain_scores_gemma":[0.99699223,0.00087431807,0.0010017398,0.00041518878,0.00039230994,0.00032418303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066144054,0.00013413385,0.00021038699,0.000906355,0.00029044898,0.0004867801,0.00024921732,0.00016094954,0.00069252186],"category_scores_gemma":[0.0032372924,0.00015530961,0.00012344895,0.00047270145,0.00040639582,0.0003283798,0.0005724481,0.00012583508,0.00015533966],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010688823,0.0000071305485,0.99237084,0.000004213677,0.00003363121,0.000015780124,0.00017913592,0.0005000455,0.0049201255,0.00009965597,0.000045054163,0.001717512],"study_design_scores_gemma":[0.0000012411958,0.000011960115,0.9977621,0.000001141173,0.000008563443,0.000019032143,0.000063290856,0.0013527567,0.00065044966,0.00006113604,0.00006599528,0.000002277707],"about_ca_topic_score_codex":0.0045455764,"about_ca_topic_score_gemma":0.0042297593,"teacher_disagreement_score":0.0045455764,"about_ca_system_score_codex":0.00029887512,"about_ca_system_score_gemma":0.00008630668,"threshold_uncertainty_score":0.00903821},"labels":[],"label_agreement":null},{"id":"W2921558679","doi":"10.3847/1538-4357/ab0f30","title":"The Redshift Dependence of the Alcock–Paczynski Effect: Cosmological Constraints from the Current and Next Generation Observations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"National Natural Science Foundation of China","keywords":"Redshift; Dark energy; Galaxy; Universe; Cosmology; Cluster analysis; Equation of state; Galaxy cluster; Current (fluid)","score_opus":0.022794503072064914,"score_gpt":0.23256088665304583,"score_spread":0.20976638358098093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2921558679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9664216,0.00065806776,0.022440676,0.0007358572,0.000022541088,0.000012274442,0.00071245857,0.00019600059,0.008800551],"genre_scores_gemma":[0.998226,0.00006345521,0.0012192838,0.000047760703,0.000020083064,0.0000037743991,0.00019247766,0.000022026366,0.00020517394],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.998825,0.0002389074,0.000058835594,0.00041911006,0.00029229035,0.0001657934],"domain_scores_gemma":[0.9875907,0.0059381556,0.0026270149,0.0022149242,0.0007845571,0.00084466726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0030451007,0.00035073556,0.00043828052,0.0016094376,0.00058566773,0.0015065101,0.0009821773,0.0004799403,0.00336784],"category_scores_gemma":[0.01255914,0.00029046033,0.00045687016,0.0010526798,0.001348054,0.0021972498,0.0015599672,0.00096406153,0.00035286305],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031996248,0.00005332896,0.8968562,0.00013631671,0.00041452685,0.0004947671,0.00044647531,0.010762673,0.015893698,0.029106654,0.002037384,0.04347809],"study_design_scores_gemma":[0.000031465133,0.000045106037,0.9368419,0.000045734105,0.000208964,0.00029309365,0.00019001999,0.043820396,0.005862251,0.009863403,0.0027328625,0.00006490092],"about_ca_topic_score_codex":0.011078454,"about_ca_topic_score_gemma":0.010407371,"teacher_disagreement_score":0.011078454,"about_ca_system_score_codex":0.0003831992,"about_ca_system_score_gemma":0.00039746024,"threshold_uncertainty_score":0.02202791},"labels":[],"label_agreement":null},{"id":"W2921923599","doi":"10.3847/1538-4357/ab2879","title":"The Redshifted 21 cm Signal in the EDGES Low-band Spectrum","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Redshift; Amplitude; Cosmology; COSMIC cancer database; Observational cosmology; Absorption (acoustics); Residual; Spectral line; Absorption spectroscopy","score_opus":0.006285703448429339,"score_gpt":0.2062643950903431,"score_spread":0.19997869164191379,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2921923599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9665841,0.00047056552,0.010874095,0.00068227015,0.00007792583,0.000007757478,0.002425123,0.00049891724,0.018379366],"genre_scores_gemma":[0.9954586,0.00009107726,0.0021997944,0.00014140156,0.000023553535,0.0000027298734,0.0011133928,0.00009302154,0.0008764822],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997769,0.000026536301,0.0000087007475,0.000072681425,0.000058661622,0.000056568842],"domain_scores_gemma":[0.9990988,0.00019100499,0.0002611117,0.00016855795,0.00017782072,0.00010276782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005066565,0.00028486075,0.00012573853,0.0007008924,0.00033683333,0.00068050314,0.000242685,0.00030470188,0.0031948953],"category_scores_gemma":[0.0012109753,0.00010456173,0.00023928865,0.00072665233,0.00031118613,0.00045961904,0.0005294101,0.00040990612,0.0007494204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012741041,0.00008701479,0.759528,0.00025471256,0.00021506219,0.0008357505,0.0017526093,0.0022439517,0.10154845,0.023216497,0.010344281,0.09869967],"study_design_scores_gemma":[0.000012795527,0.00005453365,0.9586504,0.000035535577,0.00007717515,0.00054494065,0.00037179238,0.0027287041,0.0128089525,0.004872399,0.019810472,0.000032437412],"about_ca_topic_score_codex":0.003376847,"about_ca_topic_score_gemma":0.006706757,"teacher_disagreement_score":0.003376847,"about_ca_system_score_codex":0.00033563768,"about_ca_system_score_gemma":0.000109719935,"threshold_uncertainty_score":0.010688007},"labels":[],"label_agreement":null},{"id":"W2921970006","doi":"10.3847/1538-4357/ab0c08","title":"The Green Bank Ammonia Survey: A Virial Analysis of Gould Belt Clouds in Data Release 1","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Victoria; Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Green Bank Telescope; Virial theorem; Observatory; Turbulence; Core (optical fiber); Molecular cloud; Star formation; Telescope","score_opus":0.022362965057586035,"score_gpt":0.2741312596777712,"score_spread":0.25176829462018513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2921970006","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97409564,0.00010319551,0.00048497683,0.0000685263,0.0000044997278,0.000030593157,0.022786915,0.000096266886,0.0023294298],"genre_scores_gemma":[0.9471553,0.0000983865,0.003063144,0.000091763344,0.000013869845,0.000062469895,0.04820627,0.00006444147,0.0012443401],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979097,0.000049857634,0.000010432963,0.0000390321,0.000055548167,0.000054125827],"domain_scores_gemma":[0.9994929,0.00007831757,0.00014278959,0.00009507448,0.00007281172,0.00011812221],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003812087,0.00017909968,0.0001963432,0.0018478428,0.0003804804,0.00040551848,0.00032684059,0.00013773682,0.0018249907],"category_scores_gemma":[0.0008878878,0.00010298362,0.00024144887,0.0016031684,0.00014749152,0.00016442641,0.0007181588,0.00014945258,0.00060477795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000108452696,0.0000338695,0.97615314,0.000025855612,0.000084422776,0.000105790365,0.00017561724,0.0020892597,0.0034579965,0.0003942245,0.007941568,0.009429874],"study_design_scores_gemma":[0.000008513276,0.0000074623263,0.9949562,0.000006108583,0.0000072378407,0.00002222093,0.00008024478,0.0022416771,0.00024833166,0.000067539,0.002349243,0.000005104749],"about_ca_topic_score_codex":0.1114715,"about_ca_topic_score_gemma":0.15239756,"teacher_disagreement_score":0.1114715,"about_ca_system_score_codex":0.00064738654,"about_ca_system_score_gemma":0.00058460113,"threshold_uncertainty_score":0.22164536},"labels":[],"label_agreement":null},{"id":"W2922188800","doi":"10.3847/1538-4357/ab095b","title":"Inferred Evidence for Dark Matter Kinematic Substructure with SDSS–Gaia","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Science and Technology Facilities Council; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; European Space Agency; National Science Foundation; University of Washington; Flatiron Health; Alfred P. Sloan Foundation; Princeton University; Brookhaven National Laboratory; European Commission; U.S. Department of Energy; Research Corporation for Science Advancement","keywords":"Physics; Halo; Dark matter; Astrophysics; Substructure; Dark matter halo; Astronomy; Galactic halo; Population; Milky Way; Stars; Galaxy","score_opus":0.01017340326543836,"score_gpt":0.23104245238402135,"score_spread":0.220869049118583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2922188800","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99268943,0.00011550284,0.0013469753,0.00005914371,0.0000052092073,0.000008094413,0.0034930818,0.00020472713,0.002077951],"genre_scores_gemma":[0.9964367,0.00002366225,0.00044640453,0.0000114212535,0.0000049786436,0.0000025573734,0.002869388,0.000017998647,0.00018701208],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99953437,0.000106282016,0.00003383908,0.00013130925,0.00010671763,0.00008746039],"domain_scores_gemma":[0.9980716,0.00028110784,0.00066095224,0.00042227664,0.00029807084,0.0002660214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012215902,0.000311333,0.00031488916,0.0023303619,0.00026270002,0.0010534007,0.0002361588,0.00017981407,0.0013137995],"category_scores_gemma":[0.002258508,0.0001850808,0.00042632085,0.0014976863,0.0003218177,0.0002754256,0.00063862937,0.00021701862,0.00060627563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007014065,0.000011338062,0.9925541,0.000012302163,0.00011711539,0.000034406716,0.000057810466,0.0017592482,0.0024634227,0.00031882297,0.00045099438,0.0021501677],"study_design_scores_gemma":[0.000003993767,0.00000972123,0.9928685,0.000003429411,0.000019203515,0.00003938262,0.000040144667,0.005588137,0.0006286016,0.0001413289,0.0006536123,0.000003989763],"about_ca_topic_score_codex":0.0124079995,"about_ca_topic_score_gemma":0.011564607,"teacher_disagreement_score":0.0124079995,"about_ca_system_score_codex":0.00050688395,"about_ca_system_score_gemma":0.0002359965,"threshold_uncertainty_score":0.024671555},"labels":[],"label_agreement":null},{"id":"W2922276918","doi":"10.3847/1538-4357/ab2e07","title":"Butterfly in a Cocoon, Understanding the Origin and Morphology of Globular Cluster Streams: The Case of GD-1","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Vetenskapsrådet","keywords":"Globular cluster; Physics; Butterfly; STREAMS; Morphology (biology); Cluster (spacecraft); Astrophysics; Astronomy; Horizontal branch; Astrobiology; Stars; Zoology; Ecology; Biology","score_opus":0.016860722665165244,"score_gpt":0.24221133753838842,"score_spread":0.22535061487322317,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2922276918","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99101526,0.00051454507,0.0021905517,0.00043133824,0.000012596242,0.000013140861,0.000087435255,0.000035344696,0.005699777],"genre_scores_gemma":[0.99600583,0.00021478932,0.0028664262,0.000050233033,0.000012631287,0.0000021040503,0.000062758365,0.00001402087,0.0007713013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999536,0.0000060297943,0.0000016751115,0.000016803026,0.000007589016,0.000014254913],"domain_scores_gemma":[0.9997483,0.000057082478,0.000064576845,0.00003523356,0.000035625704,0.000059206683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017110168,0.00013789951,0.00008839965,0.0009718474,0.000535547,0.00090442435,0.00024310533,0.00038960794,0.0017526095],"category_scores_gemma":[0.00097354746,0.00009462309,0.000100351055,0.0004626049,0.0009983592,0.0009725981,0.00048496836,0.00026712578,0.00021056138],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046115715,0.00005021939,0.8101635,0.00012781433,0.00005076404,0.039560933,0.010360452,0.0017908394,0.04996499,0.02656525,0.002641487,0.05826257],"study_design_scores_gemma":[0.00001803796,0.00007015119,0.88873565,0.00011602687,0.00005363895,0.02515895,0.014776951,0.013960946,0.007886062,0.016539987,0.03264392,0.000039590734],"about_ca_topic_score_codex":0.016866896,"about_ca_topic_score_gemma":0.02362465,"teacher_disagreement_score":0.016866896,"about_ca_system_score_codex":0.00065944204,"about_ca_system_score_gemma":0.00024919925,"threshold_uncertainty_score":0.033537447},"labels":[],"label_agreement":null},{"id":"W2922352917","doi":"10.3847/1538-4357/ab125a","title":"The XMM-Newton/HST View of the Obscuring Outflow in the Seyfert Galaxy Mrk 335 Observed at Extremely Low X-Ray Flux","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Outflow; Galaxy; Flux (metallurgy); Ionization; Spectral line; Space Telescope Imaging Spectrograph; Accretion (finance); Absorption (acoustics)","score_opus":0.0196692238320537,"score_gpt":0.22079837958550236,"score_spread":0.20112915575344867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2922352917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9790248,0.00058511685,0.0010210508,0.0002437007,0.000024452167,0.000019940157,0.0018389953,0.00048119106,0.016760707],"genre_scores_gemma":[0.9948431,0.00018583064,0.0013987826,0.00008185361,0.00005204927,0.0000073031197,0.0014079174,0.00004754753,0.0019755233],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999702,0.0000020967336,0.0000015058054,0.000007706514,0.000010307195,0.000008234778],"domain_scores_gemma":[0.9998504,0.000008612719,0.00005010068,0.000012850231,0.000021008667,0.000057080902],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000082435115,0.00025168085,0.00014570313,0.001394227,0.00028284485,0.00043443227,0.00020322631,0.00036066672,0.004580512],"category_scores_gemma":[0.000103362305,0.0001526862,0.00018824471,0.00044921777,0.00017494857,0.0002616881,0.00031052966,0.00034915988,0.0011373883],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007480711,0.0003486074,0.4885808,0.00032545265,0.0001627902,0.011454743,0.0015750325,0.004428902,0.431521,0.0039020681,0.01070759,0.046244968],"study_design_scores_gemma":[0.000009482362,0.00006495133,0.99289215,0.000016988191,0.000011934052,0.0008068653,0.000106859145,0.0021508099,0.00109908,0.0001249148,0.0027116304,0.0000042026913],"about_ca_topic_score_codex":0.003491488,"about_ca_topic_score_gemma":0.0048635225,"teacher_disagreement_score":0.004580512,"about_ca_system_score_codex":0.0002483847,"about_ca_system_score_gemma":0.00008938879,"threshold_uncertainty_score":0.015323281},"labels":[],"label_agreement":null},{"id":"W2922364607","doi":"10.3847/1538-4357/ab2bfb","title":"Can a Machine Learn the Outcome of Planetary Collisions?","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Space Science and Extraterrestrial Life","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Gradient boosting; Outcome (game theory); Collision; Boosting (machine learning); Planet; Focus (optics); Gaussian process; Set (abstract data type)","score_opus":0.01543755694405414,"score_gpt":0.2548111185196703,"score_spread":0.23937356157561618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2922364607","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3826474,0.00364678,0.5811674,0.018587187,0.0007625743,0.00009041732,0.0009796234,0.0015583696,0.010560251],"genre_scores_gemma":[0.9422265,0.00093783584,0.052245516,0.00075557496,0.00041908908,0.00006322262,0.00064791285,0.00010902034,0.0025952994],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995759,0.00016050838,0.000018088958,0.0001345896,0.000055285265,0.00005555354],"domain_scores_gemma":[0.9950329,0.003570879,0.00034722075,0.0005411153,0.0003592857,0.0001486526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019987044,0.00054555683,0.0009057882,0.00063181494,0.00046786293,0.0013148079,0.0011977918,0.0019753869,0.0024922974],"category_scores_gemma":[0.014901058,0.0003488428,0.0005428396,0.00046361645,0.0010834798,0.0045175897,0.0006799709,0.001990726,0.0010529582],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032557445,0.00029912568,0.034764323,0.00035373005,0.00025951414,0.00017249095,0.00023224347,0.73892796,0.0023569535,0.05133087,0.010814734,0.16016245],"study_design_scores_gemma":[0.000013892153,0.00004493766,0.0017740896,0.000022805965,0.000014014816,0.000040784063,0.000042634918,0.9003942,0.00064568245,0.09563252,0.0013593808,0.000015037669],"about_ca_topic_score_codex":0.0020701892,"about_ca_topic_score_gemma":0.0012876942,"teacher_disagreement_score":0.0024922974,"about_ca_system_score_codex":0.0004820123,"about_ca_system_score_gemma":0.0006493218,"threshold_uncertainty_score":0.010570288},"labels":[],"label_agreement":null},{"id":"W2922533294","doi":"10.3847/1538-4357/ab064a","title":"HARPS-N Solar RVs Are Dominated by Large, Bright Magnetic Regions","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Heliophysics Division; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Université de Genève; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; California Institute of Technology; European Commission; Queen's University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; NASA Exoplanet Science Institute; Harvard University; National Aeronautics and Space Administration; John Templeton Foundation; Smithsonian Institution; National Science Foundation","keywords":"Physics; Photometry (optics); Exoplanet; Light curve; Astrophysics; Stars","score_opus":0.005189322895503324,"score_gpt":0.20030251115119663,"score_spread":0.1951131882556933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2922533294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98594505,0.0001823358,0.0018201187,0.00004867041,0.000009884505,0.000012378795,0.0038262517,0.0005800204,0.0075752847],"genre_scores_gemma":[0.99129266,0.0000568262,0.001129922,0.000029060266,0.000012801506,0.000009240316,0.006366649,0.00012956577,0.0009733362],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998093,0.000016400105,0.00000943962,0.00008993002,0.000038773254,0.000036176483],"domain_scores_gemma":[0.99951804,0.000088056186,0.00014756173,0.00007796555,0.00008382467,0.00008455901],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017845463,0.00026924547,0.0002925726,0.0008455491,0.00031737806,0.00088822166,0.0002183251,0.00014333529,0.0032905592],"category_scores_gemma":[0.0008276354,0.00016046807,0.00021481708,0.00063121517,0.0002257859,0.00038073745,0.0004902334,0.0001571952,0.0011553873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041697623,0.000045610766,0.90139574,0.00011090908,0.00014426338,0.0007733916,0.00032877072,0.0029623236,0.037089393,0.0008165878,0.011681669,0.044234317],"study_design_scores_gemma":[0.000021076861,0.000028411261,0.9847409,0.000014686306,0.000027593525,0.00041159606,0.0001661903,0.004829337,0.0040807654,0.00049051066,0.0051807757,0.000008142012],"about_ca_topic_score_codex":0.003403096,"about_ca_topic_score_gemma":0.005981708,"teacher_disagreement_score":0.003403096,"about_ca_system_score_codex":0.00019158305,"about_ca_system_score_gemma":0.00010875039,"threshold_uncertainty_score":0.011008024},"labels":[],"label_agreement":null},{"id":"W2924180482","doi":"10.3847/1538-4357/ab05cd","title":"Sub-Eddington Supermassive Black Hole Activity in Fornax Early-type Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Virgo Cluster; Supermassive black hole; Fornax Cluster; Galaxy; Active galactic nucleus; Luminosity; Black hole (networking); Galaxy cluster","score_opus":0.007163987520674194,"score_gpt":0.21377624233147707,"score_spread":0.2066122548108029,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2924180482","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999663,0.000045191566,0.000033130873,0.000003698973,4.0959264e-7,0.0000014322225,0.000037015223,0.0000036707438,0.00021247799],"genre_scores_gemma":[0.99972874,0.000019706707,0.000046424877,0.0000028763814,0.000002371824,0.000001246485,0.000086210835,0.0000011359056,0.00011133448],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999806,0.000029345303,0.000010655039,0.000068379566,0.00003638503,0.000049397164],"domain_scores_gemma":[0.9991572,0.00014614269,0.00035306934,0.00011048548,0.000058248857,0.00017488904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035454688,0.00025799312,0.00026972694,0.0011437257,0.0002591165,0.0006532942,0.00030087295,0.00025834193,0.0011516277],"category_scores_gemma":[0.0006982031,0.00012693187,0.00021067787,0.00036566093,0.00038705376,0.00033426966,0.00044895455,0.0001533644,0.00030606735],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000087263455,0.000020198418,0.98861724,0.000008440777,0.00002447106,0.00006278264,0.0002695705,0.000060100287,0.008971161,0.000058020883,0.000024805937,0.001796125],"study_design_scores_gemma":[6.8116856e-7,0.00002074859,0.9996045,8.404998e-7,0.0000026413359,0.00004474243,0.000043521595,0.000043174383,0.00019157521,0.0000090747835,0.000037730373,6.6993806e-7],"about_ca_topic_score_codex":0.0023311644,"about_ca_topic_score_gemma":0.002106077,"teacher_disagreement_score":0.0023311644,"about_ca_system_score_codex":0.00020993533,"about_ca_system_score_gemma":0.00008846432,"threshold_uncertainty_score":0.004635155},"labels":[],"label_agreement":null},{"id":"W2924509630","doi":"10.3847/1538-4357/ab0b43","title":"Chemical Abundances of Main-sequence, Turnoff, Subgiant, and Red Giant Stars from APOGEE Spectra. II. Atomic Diffusion in M67 Stars","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Stars; Red giant; Abundance (ecology); Open cluster; Spectral line; Red-giant branch; Abundance of the chemical elements; Stellar evolution; Giant star; Diffusion","score_opus":0.0077815778100704565,"score_gpt":0.21017074636045377,"score_spread":0.2023891685503833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2924509630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999374,0.00006378831,0.000054869168,0.0000050273693,7.036785e-7,0.000001000103,0.00032710444,0.000007806766,0.00016566431],"genre_scores_gemma":[0.9977022,0.0000595341,0.00020689768,0.0000068038494,0.0000027774956,0.00000271241,0.0018584352,0.000011240462,0.00014950323],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999454,0.0000048891407,0.0000039926504,0.000020996442,0.000013453866,0.000011321223],"domain_scores_gemma":[0.99973685,0.000043176475,0.00009196419,0.000031200678,0.000039762035,0.000057008434],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015225861,0.00029600764,0.00020361287,0.0014438865,0.00021680396,0.0003706591,0.0001704068,0.00024707476,0.0007566376],"category_scores_gemma":[0.00041807868,0.00012620604,0.0002373271,0.00059328816,0.00022087997,0.00017502115,0.00039191754,0.00012126879,0.00037855795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026330238,0.000025266823,0.94693744,0.00007646915,0.00007911806,0.00013747838,0.0003750746,0.001653845,0.040686835,0.00024241803,0.00043030636,0.009092389],"study_design_scores_gemma":[0.000005867087,0.000027046342,0.99618775,0.0000042137954,0.000012581748,0.00008597589,0.00009496554,0.0015488062,0.0014983632,0.00005745599,0.00047274318,0.0000041824865],"about_ca_topic_score_codex":0.0034815278,"about_ca_topic_score_gemma":0.005039065,"teacher_disagreement_score":0.0034815278,"about_ca_system_score_codex":0.0003259149,"about_ca_system_score_gemma":0.00008175661,"threshold_uncertainty_score":0.006922543},"labels":[],"label_agreement":null},{"id":"W2924510439","doi":"10.3847/1538-4357/ab0d1e","title":"New Insights into the Physical Conditions and Internal Structure of a Candidate Proto-globular Cluster","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Molecular cloud; Milky Way; Cluster (spacecraft); RADIUS; Star cluster; Stars; Galaxy","score_opus":0.003756301479657454,"score_gpt":0.23088972441407818,"score_spread":0.22713342293442074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2924510439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984333,0.00004601453,0.0004472531,0.000031784453,0.0000014188281,0.0000016814472,0.00005241195,0.000012133525,0.0009739074],"genre_scores_gemma":[0.9993923,0.0000115072935,0.00030399018,0.000009870901,0.00000215144,7.2649925e-7,0.00008253217,0.0000028281438,0.00019419189],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999691,0.0000018577481,7.6405234e-7,0.000010373374,0.000007457907,0.000010453008],"domain_scores_gemma":[0.99988353,0.00001397362,0.000022511162,0.000013582463,0.000020515128,0.000045911518],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007478601,0.00008506156,0.00013573133,0.0003572495,0.00055160996,0.00043577945,0.00029210545,0.00023347019,0.0017105271],"category_scores_gemma":[0.00019084683,0.00011531255,0.00010520361,0.00033693065,0.0004075508,0.00024781225,0.0003445563,0.00019467314,0.00022825539],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045324082,0.00009550999,0.65955126,0.000065392436,0.00006144035,0.001790441,0.0013699236,0.0063046184,0.3142893,0.0041248924,0.0012722441,0.010621719],"study_design_scores_gemma":[0.00000992985,0.00003520763,0.98339397,0.00000658486,0.000012810806,0.0002970504,0.00048076935,0.009382957,0.0046965857,0.0006076866,0.0010662572,0.0000102700815],"about_ca_topic_score_codex":0.0067380867,"about_ca_topic_score_gemma":0.011351339,"teacher_disagreement_score":0.0067380867,"about_ca_system_score_codex":0.00067372195,"about_ca_system_score_gemma":0.0001440431,"threshold_uncertainty_score":0.013397753},"labels":[],"label_agreement":null},{"id":"W2924752088","doi":"10.3847/1538-4357/ab50bb","title":"Anisotropic Mass Segregation in Rotating Globular Clusters","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Globular cluster; Mass segregation; Anisotropy; Mass distribution; Stars; Star cluster; Population; Stellar mass; Stellar population; Stellar evolution","score_opus":0.007280873496023608,"score_gpt":0.21535870526487402,"score_spread":0.20807783176885042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2924752088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970687,0.000034416644,0.0014758845,0.00005249063,0.000009730257,0.000007273795,0.000036687026,0.000032610646,0.0012821307],"genre_scores_gemma":[0.9992362,0.000022182205,0.00048905425,0.00001357635,0.000005482444,0.0000048333145,0.000040486375,0.000011113544,0.00017696896],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998723,0.000030466004,0.00000523883,0.000023715682,0.000026462634,0.00004174723],"domain_scores_gemma":[0.99949384,0.000097481636,0.000107433705,0.00007278672,0.00008760101,0.00014079011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043975425,0.00033644176,0.00044407524,0.00046176542,0.0006639665,0.0007420046,0.00064750813,0.00044450792,0.0008254644],"category_scores_gemma":[0.0020158044,0.00023326214,0.00040800052,0.00036610724,0.0008693397,0.0005154391,0.0007846566,0.00031597295,0.00012471591],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018075669,0.000072408286,0.03110651,0.00002504469,0.000086941654,0.00030166467,0.00019412789,0.9523066,0.007757089,0.0055637383,0.00049371144,0.0019113143],"study_design_scores_gemma":[0.00007424286,0.00005615846,0.013012774,0.0000045421875,0.000018154149,0.00004450854,0.0000781574,0.9839627,0.00085092714,0.0015950898,0.00028682072,0.000015833635],"about_ca_topic_score_codex":0.017811362,"about_ca_topic_score_gemma":0.0063339253,"teacher_disagreement_score":0.017811362,"about_ca_system_score_codex":0.0008131783,"about_ca_system_score_gemma":0.00058873784,"threshold_uncertainty_score":0.03541535},"labels":[],"label_agreement":null},{"id":"W2924910994","doi":"10.3847/1538-4357/ab39e4","title":"1ES 1927+654: An AGN Caught Changing Look on a Timescale of Months","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":188,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Chinese Academy of Sciences; Center for Cosmology and Astroparticle Physics, Ohio State University; Liverpool John Moores University; National Natural Science Foundation of China; Jet Propulsion Laboratory; Chinese Academy of Sciences South America Center for Astronomy; W. M. Keck Foundation; Space Telescope Science Institute; Villum Fonden; Queen's University; Ohio State University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; Israel Science Foundation; Queen's University Belfast; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Balmer series; Active galactic nucleus; Emission spectrum; Galaxy; Luminosity; Basso continuo; Spectroscopy; Spectral line","score_opus":0.005331601126172174,"score_gpt":0.20388809614366224,"score_spread":0.19855649501749006,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2924910994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99876547,0.00003878449,0.00014096458,0.00006350561,0.000009837756,0.0000032282655,0.00012879641,0.000013482727,0.00083588],"genre_scores_gemma":[0.9986959,0.000016195898,0.00016659388,0.000036381807,0.000016623908,0.0000031121544,0.00029468184,0.000005223781,0.0007651736],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999447,0.0000050449266,0.0000018731248,0.000016688738,0.000013275055,0.000018495808],"domain_scores_gemma":[0.9998161,0.000020901993,0.000059210757,0.00001330474,0.00001844969,0.000071988354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014271734,0.00017081121,0.00020171684,0.00033242328,0.00042426272,0.00045091764,0.00022398989,0.00032539273,0.0017299931],"category_scores_gemma":[0.00027726436,0.00007626383,0.00013260776,0.00021163783,0.0002060805,0.00023186672,0.00035562064,0.0003655182,0.00039409634],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004769492,0.00038456096,0.9195732,0.00004430349,0.000104021165,0.0055063176,0.0006531382,0.0026341563,0.048273332,0.0016552749,0.0034652564,0.017229505],"study_design_scores_gemma":[0.000023089917,0.0003989652,0.98284596,0.000009989799,0.000033522054,0.0018684472,0.00083089824,0.004927644,0.0022916,0.0007827471,0.0059643723,0.000022745191],"about_ca_topic_score_codex":0.0028031908,"about_ca_topic_score_gemma":0.004747369,"teacher_disagreement_score":0.0028031908,"about_ca_system_score_codex":0.00033570678,"about_ca_system_score_gemma":0.000092642695,"threshold_uncertainty_score":0.005787432},"labels":[],"label_agreement":null},{"id":"W2925171323","doi":"10.3847/1538-4357/ab1266","title":"Line Profiles of the Calcium I Resonance Line in Cool Metal-polluted White Dwarfs","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Line (geometry); Atmosphere (unit); Spectral line; Resonance (particle physics); Dipole; Stellar atmosphere; Helium","score_opus":0.013147606792720205,"score_gpt":0.24782162347966624,"score_spread":0.23467401668694604,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2925171323","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960543,0.000036283916,0.0029355574,0.000015991078,0.000002245413,0.000004257889,0.00014507283,0.00012176275,0.00068444153],"genre_scores_gemma":[0.9990908,0.000013680108,0.00063326745,0.000004039138,8.9321713e-7,0.0000019256008,0.00011438768,0.00001179623,0.00012930771],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999535,0.000006770479,0.0000024193089,0.000017142705,0.000011099545,0.000009050204],"domain_scores_gemma":[0.99984527,0.000044219967,0.000030000072,0.000015947026,0.00003756348,0.000026998378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016566194,0.00022707824,0.00016050297,0.00041974435,0.00024869203,0.00036111343,0.00040260996,0.00033884807,0.0006464876],"category_scores_gemma":[0.0004895082,0.00011126526,0.00026053793,0.00025685137,0.0002358669,0.0002314228,0.00027614555,0.00017039574,0.00013236067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065782684,0.00016886367,0.40787268,0.00012116566,0.0001324428,0.00078591803,0.0007582271,0.36044782,0.2092641,0.0038468712,0.0006881876,0.015255927],"study_design_scores_gemma":[0.00009537515,0.00018559746,0.17836899,0.00001539757,0.00004534108,0.00016265099,0.00033388604,0.77414006,0.044238295,0.0012096178,0.0011665605,0.000038229293],"about_ca_topic_score_codex":0.0072959675,"about_ca_topic_score_gemma":0.003743236,"teacher_disagreement_score":0.0072959675,"about_ca_system_score_codex":0.00042670444,"about_ca_system_score_gemma":0.00015923863,"threshold_uncertainty_score":0.014506996},"labels":[],"label_agreement":null},{"id":"W2925202991","doi":"10.3847/1538-4357/ab20cb","title":"Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015–2017 LIGO Data","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":118,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Human Resource Development; Office of Naval Research; Science and Technology Facilities Council; NASA Headquarters; ICTP South American Institute for Fundamental Research; Istituto Nazionale di Fisica Nucleare; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Engineering and Physical Sciences Research Council; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; National Natural Science Foundation of China; European Commission; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; National Research Foundation; National Aeronautics and Space Administration; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; Nuclear Safety and Security Commission; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; LIGO; Gravitational wave; Pulsar; Astronomy; Astrophysics; Einstein Telescope; Harmonics; Gravitational-wave observatory; Gravitational-wave astronomy","score_opus":0.04918122121753842,"score_gpt":0.37891164427812574,"score_spread":0.3297304230605873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2925202991","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946555,0.00016263437,0.00075773656,0.00008249631,0.000010639465,0.000007955614,0.0025796455,0.000045950634,0.0016975085],"genre_scores_gemma":[0.9888136,0.0000836495,0.000800093,0.00005514887,0.000028619837,0.0000114166705,0.009737349,0.000023080791,0.00044706493],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99929357,0.000078626865,0.000059606715,0.00008122811,0.00029843376,0.00018859733],"domain_scores_gemma":[0.9975746,0.00043845395,0.0010023067,0.0003148867,0.00029786845,0.00037193025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011726448,0.00022828803,0.00038876387,0.0038737238,0.00039215165,0.0010664765,0.0003166059,0.00039320337,0.0010313586],"category_scores_gemma":[0.0032306276,0.00020641164,0.00038995594,0.0014486567,0.0004418502,0.0006592555,0.0015328148,0.0002864332,0.0005070522],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002885513,0.000075581265,0.96610206,0.00004576294,0.00013109358,0.00020051819,0.00043887572,0.0012644433,0.012542587,0.00071968784,0.0015292637,0.01666149],"study_design_scores_gemma":[0.000018718203,0.0000662538,0.9889522,0.000022862681,0.000045085006,0.00025283705,0.00016884778,0.0019405147,0.0035514426,0.00040599363,0.004549394,0.000025943427],"about_ca_topic_score_codex":0.0033312377,"about_ca_topic_score_gemma":0.0052733365,"teacher_disagreement_score":0.0038737238,"about_ca_system_score_codex":0.0005252803,"about_ca_system_score_gemma":0.00050187006,"threshold_uncertainty_score":0.0066236854},"labels":[],"label_agreement":null},{"id":"W2927107815","doi":"10.3847/1538-4357/ab1d67","title":"An Initial Overview of the Extent and Structure of Recent Star Formation within the Serpens Molecular Cloud Using Gaia Data Release 2","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Serpens; Protostar; Star formation; Molecular cloud; Stars; Population","score_opus":0.036495451280517205,"score_gpt":0.30065991080017457,"score_spread":0.2641644595196574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2927107815","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9561039,0.00081598567,0.0011971042,0.000082091035,0.000009401283,0.00004153884,0.03558438,0.00043443884,0.0057311845],"genre_scores_gemma":[0.9596477,0.0006915708,0.002936401,0.00003357147,0.000017865688,0.00001848895,0.035715763,0.0000901612,0.0008484482],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997869,0.000022894195,0.000026587155,0.00005937238,0.000057188543,0.000047006808],"domain_scores_gemma":[0.99922097,0.0001327168,0.00027158842,0.0001079021,0.00017036365,0.0000964487],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000323971,0.00025610067,0.0001733761,0.0040236474,0.00018331956,0.0006333801,0.00024221875,0.00010997793,0.0012836203],"category_scores_gemma":[0.0008629888,0.00011140881,0.0003426874,0.0029230537,0.0001312291,0.00041983835,0.000437932,0.00015756437,0.0005514459],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013331624,0.000016177197,0.97016,0.00010161692,0.00007047247,0.00014280554,0.00016594604,0.001789606,0.0048383945,0.00022908353,0.0018956958,0.020456895],"study_design_scores_gemma":[0.0000027566473,0.000013008441,0.992912,0.00001949421,0.000013381294,0.00005450201,0.00010995899,0.0011027072,0.0010967115,0.000029801675,0.004641066,0.000004614869],"about_ca_topic_score_codex":0.020343017,"about_ca_topic_score_gemma":0.027707197,"teacher_disagreement_score":0.020343017,"about_ca_system_score_codex":0.00036941157,"about_ca_system_score_gemma":0.00024966468,"threshold_uncertainty_score":0.040449202},"labels":[],"label_agreement":null},{"id":"W2928527894","doi":"10.3847/1538-4357/ab4ea5","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Initial C iv Lag Results from Four Years of Data","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Reverberation mapping; Physics; Quasar; Astrophysics; Sky; Luminosity; Redshift; Black hole (networking); Accretion (finance); Astronomy; RADIUS; Reverberation; Acoustics","score_opus":0.03548869407875876,"score_gpt":0.2555152105710159,"score_spread":0.22002651649225713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2928527894","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989687,0.00010133498,0.0005654578,0.000036081,0.0000054022103,0.000025353105,0.008857395,0.00007785518,0.0006440494],"genre_scores_gemma":[0.9608344,0.00009115232,0.0026847222,0.000027926955,0.000018782524,0.00006551057,0.03560779,0.000058453545,0.00061135145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99861383,0.00041492126,0.00011523453,0.00023391642,0.0003765452,0.0002455607],"domain_scores_gemma":[0.99368757,0.0010525003,0.0016163546,0.0014488702,0.0014907159,0.0007040317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026836274,0.00045376862,0.0002849447,0.0017708787,0.0005261853,0.0007488471,0.0004768835,0.00028552228,0.0006555145],"category_scores_gemma":[0.003865377,0.00019906448,0.0003114773,0.0017539907,0.00028319051,0.00051239977,0.0010281829,0.00032863815,0.00043865442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041881448,0.00013869508,0.9779568,0.000051302257,0.00013608448,0.00015697876,0.00047819165,0.0011727262,0.002984423,0.00008735176,0.002182134,0.0142364735],"study_design_scores_gemma":[0.000011561342,0.00007822449,0.9960179,0.00000511922,0.000022955577,0.000056955836,0.00012547127,0.0006377353,0.00085975125,0.000017429125,0.0021580108,0.000008890557],"about_ca_topic_score_codex":0.025098618,"about_ca_topic_score_gemma":0.04213261,"teacher_disagreement_score":0.025098618,"about_ca_system_score_codex":0.0005620428,"about_ca_system_score_gemma":0.00045592047,"threshold_uncertainty_score":0.04990506},"labels":[],"label_agreement":null},{"id":"W2929513547","doi":"10.3847/1538-4357/aae82e","title":"QED Phenomena in an Ultrastrong Magnetic Field. II. Electron–Positron Scattering, e<sup>±</sup>–Ion Scattering, and Relativistic Bremsstrahlung","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Bremsstrahlung; Electron; Scattering; Atomic physics; Magnetar; Positron; Magnetic field; Landau quantization; Ion; Neutron star; Nuclear physics; Quantum mechanics","score_opus":0.0061568455758367726,"score_gpt":0.2715453029439509,"score_spread":0.2653884573681141,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2929513547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78246355,0.0024909254,0.154988,0.0013338621,0.0002085986,0.00004889485,0.00007656837,0.00023995797,0.05814969],"genre_scores_gemma":[0.9895539,0.00031358883,0.006269864,0.000112470196,0.00003712133,0.000015593741,0.00002108393,0.000031499836,0.0036448773],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99981457,0.00006966868,0.0000046809237,0.000018694504,0.0000524704,0.000040036095],"domain_scores_gemma":[0.9996517,0.0001778233,0.0000663857,0.00004261142,0.000036380872,0.000025116848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054428383,0.00031306202,0.0004425472,0.0005091708,0.00062388426,0.00066814973,0.0005448776,0.00046577657,0.0019944697],"category_scores_gemma":[0.0013599927,0.00023466795,0.00036701476,0.0005162147,0.0016364853,0.0010301528,0.00072413636,0.00050248136,0.0001985023],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010127958,0.000049692044,0.0024247805,0.00010697888,0.000031092986,0.00044244865,0.00023286407,0.10188682,0.0150911175,0.8709591,0.0006123755,0.0080614975],"study_design_scores_gemma":[0.00006296969,0.000065575536,0.0040828823,0.000014250822,0.000015077843,0.00022657882,0.00008293336,0.6794864,0.0062362417,0.307118,0.002580653,0.000028436603],"about_ca_topic_score_codex":0.0018872954,"about_ca_topic_score_gemma":0.0010597642,"teacher_disagreement_score":0.0019944697,"about_ca_system_score_codex":0.0012003616,"about_ca_system_score_gemma":0.00029240892,"threshold_uncertainty_score":0.0087093115},"labels":[],"label_agreement":null},{"id":"W2930378756","doi":"10.3847/1538-4357/ab21b9","title":"The Coevolution of Massive Quiescent Galaxies and Their Dark Matter Halos over the Last 6 Billion Years","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Smithsonian Astrophysical Observatory","keywords":"Physics; Astrophysics; Dark matter; Halo; Galaxy; Velocity dispersion; Stellar mass; Dark matter halo; Virial mass; Stellar population; Astronomy; Galaxy formation and evolution; Star formation","score_opus":0.004099928577985187,"score_gpt":0.18845565572882841,"score_spread":0.18435572715084322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2930378756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989662,0.00015632664,0.00017743245,0.00008411495,0.0000016120595,9.44667e-7,0.00015913286,0.0000093007675,0.0004448979],"genre_scores_gemma":[0.999595,0.00004620808,0.000068098874,0.000010462918,0.0000023386526,6.027801e-7,0.00017117882,0.0000026945515,0.000103375954],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998987,0.000023748764,0.0000070637193,0.00003413846,0.000015526295,0.00002090922],"domain_scores_gemma":[0.9985197,0.0003345111,0.0006192439,0.00013563245,0.00013261099,0.00025828366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00077500945,0.0001575875,0.00015734021,0.0008295651,0.00034044543,0.0009641768,0.00025432947,0.00036936914,0.00095347624],"category_scores_gemma":[0.0032511742,0.00015498401,0.00029983322,0.00061481615,0.0005450509,0.00089496514,0.00063353166,0.00025531757,0.00015348481],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000078955774,0.000017191838,0.98302,0.000016020262,0.00009252061,0.00011429566,0.00032177093,0.006282336,0.0023010315,0.0018157716,0.00027951703,0.0056606093],"study_design_scores_gemma":[0.000004648048,0.00003277449,0.98304325,0.000008991205,0.00003022024,0.00012322553,0.00018159694,0.014091465,0.00049649633,0.0008949514,0.0010826502,0.000009664055],"about_ca_topic_score_codex":0.009953047,"about_ca_topic_score_gemma":0.010973692,"teacher_disagreement_score":0.009953047,"about_ca_system_score_codex":0.00062935473,"about_ca_system_score_gemma":0.00015716748,"threshold_uncertainty_score":0.019790232},"labels":[],"label_agreement":null},{"id":"W2930652491","doi":"10.3847/1538-4357/ab391d","title":"BICEP2/Keck Array XI: Beam Characterization and Temperature-to-Polarization Leakage in the BK15 Data Set","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Advanced Research; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Cosmic microwave background; CMB cold spot; Planck; Physics; Polarization (electrochemistry); Astrophysics; Cosmic background radiation; Leakage (economics); Computational physics; Optics; Anisotropy","score_opus":0.010140957825911923,"score_gpt":0.24881300938694126,"score_spread":0.23867205156102933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2930652491","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9861399,0.00010819662,0.0041095777,0.00008914401,0.000013514373,0.000012897251,0.007607593,0.00022659323,0.0016925719],"genre_scores_gemma":[0.97423065,0.0000349789,0.0046914155,0.00008555185,0.000011028549,0.000035302328,0.020516407,0.000104954765,0.00028965762],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9985033,0.00043401134,0.00011551995,0.00042465853,0.00032305717,0.00019940328],"domain_scores_gemma":[0.9972621,0.0005515403,0.00044176637,0.0009319323,0.0005968127,0.0002158888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025078275,0.00037063455,0.00045401003,0.0009761843,0.0004454935,0.0010169874,0.0007013438,0.0003828094,0.0012850417],"category_scores_gemma":[0.0032641122,0.00034726338,0.0004264887,0.0019511516,0.00041002803,0.0007069844,0.0012055971,0.00043135736,0.0005518605],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014673873,0.00012807516,0.9121733,0.00010871309,0.0007530763,0.00033002853,0.00045246002,0.021346997,0.029360067,0.0023051277,0.007278286,0.024296552],"study_design_scores_gemma":[0.00006564254,0.000051688687,0.95648634,0.000025123301,0.00006968712,0.00022215948,0.00013952938,0.029358458,0.009280033,0.0006623399,0.0035934434,0.000045606972],"about_ca_topic_score_codex":0.0069691427,"about_ca_topic_score_gemma":0.009269804,"teacher_disagreement_score":0.0069691427,"about_ca_system_score_codex":0.00034983558,"about_ca_system_score_gemma":0.00034919134,"threshold_uncertainty_score":0.013857186},"labels":[],"label_agreement":null},{"id":"W2931769884","doi":"10.3847/1538-4357/ab67bd","title":"Multiphase Gas Flows in the Nearby Seyfert Galaxy ESO428–G014. Paper I","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Institutes of Natural Sciences; National Astronomical Observatory of Japan; European Southern Observatory; Institut sur la Nutrition et les Aliments Fonctionnels; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Outflow; RADIUS; Galaxy; Line (geometry); Conical surface; Spiral galaxy; Geometry","score_opus":0.010252847479684614,"score_gpt":0.216318682541189,"score_spread":0.2060658350615044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2931769884","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992963,0.000025802457,0.00004786082,0.000011390263,0.0000012310379,0.0000015739015,0.000048342576,0.000010045202,0.0005574126],"genre_scores_gemma":[0.99902284,0.00003194704,0.00021289242,0.000008592239,0.0000075008343,0.000002885735,0.00029172606,0.000004237789,0.00041737643],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996924,0.00000291414,0.0000012560627,0.000010141883,0.000006185919,0.000010231765],"domain_scores_gemma":[0.99994063,0.000006441571,0.000017403823,0.000005084964,0.000006039822,0.000024358831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000054136544,0.00019375353,0.00013393971,0.0007940071,0.0002102392,0.0003679756,0.00019279026,0.00022222176,0.0014398935],"category_scores_gemma":[0.00013365482,0.00010760619,0.00010205948,0.000292855,0.00014718903,0.00028631993,0.00031521264,0.00010149406,0.00023548177],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005965721,0.00031615008,0.7529949,0.00008194082,0.000115379444,0.0026210349,0.0010413574,0.00532605,0.19945367,0.0015695082,0.0013805352,0.034502883],"study_design_scores_gemma":[0.00003559678,0.000109785906,0.98638386,0.000006201617,0.00001870247,0.0003288858,0.00027056324,0.0075884163,0.0028495938,0.00046054652,0.0019394144,0.000008311138],"about_ca_topic_score_codex":0.0019681773,"about_ca_topic_score_gemma":0.003119504,"teacher_disagreement_score":0.0019681773,"about_ca_system_score_codex":0.00029649993,"about_ca_system_score_gemma":0.00007926531,"threshold_uncertainty_score":0.0048169494},"labels":[],"label_agreement":null},{"id":"W2932069636","doi":"10.3847/1538-4357/ab4273","title":"Constraining Mass-transfer Histories of Blue Straggler Stars with COS Spectroscopy of White Dwarf Companions","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"White dwarf; Blue straggler; Stars; Open cluster; Cluster (spacecraft); Accretion (finance); Spectroscopy; Star cluster; Binary number","score_opus":0.008907848155069207,"score_gpt":0.2113160050866968,"score_spread":0.2024081569316276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2932069636","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99882084,0.000031724885,0.00040447144,0.0000042833167,0.0000010779071,0.0000031722782,0.00012306188,0.000018676745,0.0005927212],"genre_scores_gemma":[0.9993799,0.000013045766,0.00033799664,0.0000025172126,0.0000014479862,0.0000014429367,0.00018244135,0.000003139053,0.00007818171],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990344,0.000009763898,0.0000055090163,0.000036371093,0.000021606964,0.000023355145],"domain_scores_gemma":[0.99951875,0.00008920901,0.00015497538,0.000060399496,0.000064671156,0.00011195444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033664214,0.00023710614,0.00022912801,0.0014131671,0.00038792964,0.00046997107,0.00023077302,0.00021332523,0.00083937676],"category_scores_gemma":[0.0008558427,0.00015678759,0.0001843731,0.00066509325,0.00017181825,0.00032534247,0.00044997726,0.00012613939,0.0002275277],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011475506,0.00003456162,0.9729214,0.000016467156,0.0000357327,0.00008828869,0.00010282065,0.0029922347,0.019070968,0.00021433324,0.00013938938,0.0042689773],"study_design_scores_gemma":[0.000010985533,0.000065286964,0.9648542,0.00000807454,0.0000361292,0.00010702861,0.00016749428,0.027214853,0.006475293,0.0002759534,0.0007759514,0.000008810682],"about_ca_topic_score_codex":0.00919042,"about_ca_topic_score_gemma":0.020142058,"teacher_disagreement_score":0.00919042,"about_ca_system_score_codex":0.0003772529,"about_ca_system_score_gemma":0.0001734391,"threshold_uncertainty_score":0.01827383},"labels":[],"label_agreement":null},{"id":"W2934316731","doi":"10.3847/1538-4357/ab14ee","title":"The Evolution of the Quenching of Star Formation in Cluster Galaxies since z ∼ 1","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Cluster (spacecraft); Galaxy cluster; Star formation; Galaxy; Stellar mass; Population; Redshift; Quenching (fluorescence); Star cluster; Stellar population","score_opus":0.004561448199545567,"score_gpt":0.19695811370181163,"score_spread":0.19239666550226606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2934316731","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993975,0.00005920776,0.000036577723,0.000011047091,5.947067e-7,0.0000011987885,0.00023216482,0.000007971549,0.00025365822],"genre_scores_gemma":[0.9995727,0.000016916241,0.00002178613,0.0000037165303,0.0000016100443,8.959255e-7,0.0002942149,0.0000014748398,0.00008661294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998765,0.000013790221,0.0000064691926,0.0000405049,0.000020796339,0.000042063595],"domain_scores_gemma":[0.99835914,0.00032506586,0.0006463208,0.000119785014,0.00022399158,0.00032558892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043076463,0.00011796835,0.00019116829,0.0012357609,0.00021346012,0.0005091514,0.00024985065,0.00028881428,0.00095968606],"category_scores_gemma":[0.0017082853,0.00008928912,0.00017711359,0.00061113614,0.00028800612,0.00024191456,0.0002666835,0.0001973037,0.0002555124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000082741346,0.0000114915465,0.9950956,0.000004971853,0.000021816693,0.000025832713,0.00014247996,0.00027285866,0.0020004052,0.000077113415,0.00007837014,0.0021863016],"study_design_scores_gemma":[3.7588845e-7,0.000009192018,0.9997346,4.1375066e-7,0.0000017332522,0.000011696414,0.000016504247,0.000096512806,0.000074749216,0.0000058480814,0.000047782865,6.376443e-7],"about_ca_topic_score_codex":0.011221596,"about_ca_topic_score_gemma":0.010950892,"teacher_disagreement_score":0.011221596,"about_ca_system_score_codex":0.00042950318,"about_ca_system_score_gemma":0.00013689634,"threshold_uncertainty_score":0.022312522},"labels":[],"label_agreement":null},{"id":"W2935684590","doi":"10.3847/1538-4357/ab1b12","title":"Detection of Coherent Emission from the Bp Star HD 142990 at uGMRT Frequencies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Giant Metrewave Radio Telescope; Maser; Magnetic field; Cyclotron; Pulsar; Magnetic flux; Magnetic dipole; Flux (metallurgy); Star (game theory)","score_opus":0.010344924047570918,"score_gpt":0.20955536462425142,"score_spread":0.1992104405766805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2935684590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99579394,0.00008013967,0.000766066,0.000041022,0.0000072538965,0.00000564808,0.00024170354,0.00006576612,0.0029986016],"genre_scores_gemma":[0.9989157,0.000015949789,0.00054155476,0.000018366043,0.000009799773,0.00000350721,0.00022826728,0.0000043845525,0.00026261204],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999101,0.000011614217,0.0000036659658,0.000026736108,0.000031276046,0.000016619835],"domain_scores_gemma":[0.9998448,0.000022278635,0.00003304686,0.000018940442,0.00002215249,0.000058744597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011407375,0.00013139064,0.00009537116,0.00067655434,0.00027208586,0.00029269562,0.00018071664,0.0003221007,0.0012795372],"category_scores_gemma":[0.00030249142,0.000106536296,0.00007625859,0.00038106515,0.00015267091,0.00014477166,0.00040273624,0.00017671614,0.00034306524],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003170833,0.00010561781,0.3472435,0.000057531062,0.00007238605,0.0016080445,0.0004568138,0.00026459797,0.62728256,0.000470513,0.0010648989,0.021056475],"study_design_scores_gemma":[0.0000139003105,0.00009051322,0.9783689,0.00000884263,0.00001840479,0.0010021743,0.000076615936,0.0010174288,0.01763266,0.000098975695,0.0016653662,0.000006263551],"about_ca_topic_score_codex":0.0006734244,"about_ca_topic_score_gemma":0.0008845461,"teacher_disagreement_score":0.0012795372,"about_ca_system_score_codex":0.000118432836,"about_ca_system_score_gemma":0.00004258744,"threshold_uncertainty_score":0.004280448},"labels":[],"label_agreement":null},{"id":"W2935966402","doi":"10.3847/1538-4357/ab09f1","title":"Simulations of Water Vapor and Clouds on Rapidly Rotating and Tidally Locked Planets: A 3D Model Intercomparison","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Natural Science Foundation of China","keywords":"Circumstellar habitable zone; Exoplanet; Water vapor; Atmospheric model; Radiative transfer; Atmospheric models; Planet; Climate model; Atmosphere (unit)","score_opus":0.011784301254819635,"score_gpt":0.23167937350195328,"score_spread":0.21989507224713364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2935966402","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960439,0.000052787607,0.0012383587,0.00015507847,0.000021313195,0.000028580627,0.00053559116,0.00013402133,0.0017904986],"genre_scores_gemma":[0.9967499,0.00003548304,0.0023325526,0.000048557737,0.000009158713,0.000037907757,0.0004853977,0.000035887606,0.0002651902],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997607,0.00008574163,0.000016345906,0.000045311124,0.000037623828,0.00005424594],"domain_scores_gemma":[0.9987993,0.00074220943,0.00008619963,0.00012489884,0.00012469127,0.00012267468],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000876147,0.0007598798,0.00095674454,0.00061974267,0.00069488736,0.0010666162,0.0015361463,0.0023325824,0.001730703],"category_scores_gemma":[0.0015524043,0.0004473325,0.0014186044,0.0006951563,0.00083009334,0.00082771585,0.00084127404,0.0011380564,0.00014397883],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017846092,0.00025879435,0.008862313,0.000027286947,0.00008596637,0.00010257887,0.00006522219,0.98608243,0.0022136795,0.00039815326,0.00023724942,0.0014879787],"study_design_scores_gemma":[0.0000675715,0.00008523976,0.0029162772,0.0000032531002,0.000014754547,0.00000675381,0.000042946103,0.9958462,0.00073864154,0.00013142961,0.00013668473,0.000010267537],"about_ca_topic_score_codex":0.027249997,"about_ca_topic_score_gemma":0.01393931,"teacher_disagreement_score":0.027249997,"about_ca_system_score_codex":0.0012180076,"about_ca_system_score_gemma":0.0008624233,"threshold_uncertainty_score":0.054182768},"labels":[],"label_agreement":null},{"id":"W2936540985","doi":"10.3847/1538-4357/ab3c66","title":"Discovery and Early Evolution of ASASSN-19bt, the First TDE Detected by TESS","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Positive Living North","funders":"","keywords":"Light curve; Luminosity; Observatory; Supernova; Telescope; Flare; Black-body radiation; Flux (metallurgy); Event (particle physics)","score_opus":0.003967382723186868,"score_gpt":0.1895692521316876,"score_spread":0.18560186940850074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2936540985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99533916,0.00016037193,0.0004893538,0.000051439227,0.00002440942,0.0000129323325,0.002280971,0.00005852858,0.0015828677],"genre_scores_gemma":[0.9918031,0.0000981728,0.00084040954,0.000029512432,0.000028142353,0.0000085220945,0.0064270175,0.000013983615,0.0007512767],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977666,0.000013518715,0.00001784089,0.000058726426,0.00007897968,0.000054232532],"domain_scores_gemma":[0.99914396,0.000048462414,0.00021920088,0.000088696856,0.00021148041,0.00028817644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031431357,0.00021110114,0.00029638348,0.001648764,0.00045344885,0.0006244545,0.00018196902,0.00022626604,0.0010555222],"category_scores_gemma":[0.0006556826,0.00013650802,0.00029185103,0.0008644262,0.00028085156,0.00029447215,0.0009491321,0.00030777065,0.00040306],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022597171,0.00005116108,0.97063273,0.000035234734,0.000056051216,0.0010003505,0.00023906186,0.00031045612,0.013989705,0.0002984927,0.0017570136,0.01140376],"study_design_scores_gemma":[0.000008606955,0.000085743275,0.9871732,0.000020206882,0.000022240165,0.00090144906,0.00018190913,0.0007974063,0.002719298,0.00010549852,0.007972379,0.000011975229],"about_ca_topic_score_codex":0.006237061,"about_ca_topic_score_gemma":0.0147386445,"teacher_disagreement_score":0.006237061,"about_ca_system_score_codex":0.000489067,"about_ca_system_score_gemma":0.00025379463,"threshold_uncertainty_score":0.012401521},"labels":[],"label_agreement":null},{"id":"W2936588650","doi":"10.3847/1538-4357/ab1088","title":"Dicarbon Formation in Collisions of Two Carbon Atoms","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Gauss Centre for Supercomputing; Queen's University; Office of Science; Queen's University Belfast; National Energy Research Scientific Computing Center; Institute for Theoretical Atomic, Molecular and Optical Physics, Harvard University; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Semiclassical physics; Dipole; Ab initio; Collision; Moment (physics); Work (physics); Transition dipole moment; Molecule","score_opus":0.00798351806273175,"score_gpt":0.24346003335728023,"score_spread":0.23547651529454847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2936588650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993682,0.00013648903,0.0024663797,0.000031894197,0.00001397477,0.000014448798,0.00007102079,0.000034148627,0.00354954],"genre_scores_gemma":[0.99895334,0.00006293989,0.00049840356,0.000010009323,0.0000032115338,0.000008701179,0.00006747282,0.000008280897,0.00038761593],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996413,0.00005720896,0.000013104086,0.00007514557,0.00009246686,0.000120768585],"domain_scores_gemma":[0.9992323,0.0003950783,0.00013327585,0.00007228593,0.00009362232,0.00007343071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00070053886,0.0005118147,0.00059414544,0.0008913149,0.0009548413,0.00077657006,0.00095235603,0.00056592334,0.0021388035],"category_scores_gemma":[0.0014820385,0.00028084056,0.00045540463,0.00088153814,0.000628515,0.00054526544,0.000713112,0.00041300003,0.00015482566],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011269146,0.00040607265,0.05322118,0.00045309533,0.00033451334,0.0023649824,0.0009585321,0.75525445,0.09096514,0.07710948,0.00086275704,0.016942909],"study_design_scores_gemma":[0.00017514473,0.00038002696,0.033570167,0.000025159521,0.00007582707,0.00062809786,0.0002635286,0.8805362,0.07379695,0.009000306,0.0014350346,0.00011364661],"about_ca_topic_score_codex":0.004265169,"about_ca_topic_score_gemma":0.0026526493,"teacher_disagreement_score":0.004265169,"about_ca_system_score_codex":0.0017366847,"about_ca_system_score_gemma":0.0005742353,"threshold_uncertainty_score":0.012600601},"labels":[],"label_agreement":null},{"id":"W2936596612","doi":"10.3847/1538-4357/ab1b23","title":"The JCMT BISTRO Survey: The Magnetic Field of the Barnard 1 Star-forming Region","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Dalhousie University; University of Manitoba; Herzberg Institute of Astrophysics; Western University; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"National Key Research and Development Program of China; National Research Foundation; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Research Foundation of Korea; National Aeronautics and Space Administration; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; Universities Space Research Association; National Natural Science Foundation of China; Canadian Space Agency; Academia Sinica","keywords":"Magnetic field; Polarization (electrochemistry); James Clerk Maxwell Telescope; Molecular cloud; Magnetic energy; Turbulence; Amplitude; Linear polarization","score_opus":0.010377877010904783,"score_gpt":0.23076123480591587,"score_spread":0.2203833577950111,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2936596612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964049,0.000097049604,0.00012077027,0.00006298748,0.000004781292,0.0000069360435,0.0010852892,0.000048686226,0.00216853],"genre_scores_gemma":[0.997378,0.000052186468,0.00028272122,0.000040234994,0.000014923567,0.0000035980788,0.0018248929,0.000011002679,0.0003925345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990165,0.0000068145196,0.0000032889347,0.00002471003,0.00004057245,0.000022974167],"domain_scores_gemma":[0.999645,0.000016872882,0.00013301581,0.000025135705,0.000058881873,0.000121170044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000107837936,0.00012349487,0.00016604702,0.0010480463,0.00030946216,0.00030516993,0.0002366109,0.00017951103,0.0014301396],"category_scores_gemma":[0.0003045462,0.0000741163,0.00007396838,0.00044687692,0.0001260723,0.00014331807,0.0003861624,0.00019373838,0.00038811882],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015098458,0.000076138196,0.94442844,0.000036334775,0.00005684179,0.00037019947,0.00035564357,0.0008144362,0.03156086,0.00036416476,0.0035332956,0.018252652],"study_design_scores_gemma":[0.000004398024,0.000009550419,0.9975038,0.0000034634782,0.0000044925587,0.000068488676,0.000044980734,0.00066646235,0.00045144258,0.000016590626,0.0012243263,0.000002057836],"about_ca_topic_score_codex":0.02533612,"about_ca_topic_score_gemma":0.037910882,"teacher_disagreement_score":0.02533612,"about_ca_system_score_codex":0.0003381712,"about_ca_system_score_gemma":0.0001959499,"threshold_uncertainty_score":0.05037731},"labels":[],"label_agreement":null},{"id":"W2936599825","doi":"10.3847/1538-4357/ab2914","title":"Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. I. Observations, Kinematics, and Cold Dark Matter Halo Fits","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":110,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute","keywords":"Galaxy; RADIUS; Velocity dispersion; Dark matter; Stellar kinematics; Halo; Irregular galaxy; Dwarf galaxy; Effective radius; Dark matter halo","score_opus":0.009371057131399376,"score_gpt":0.19927614771872676,"score_spread":0.18990509058732738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2936599825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99880564,0.000079274745,0.000119518896,0.00001164775,0.0000012569676,0.0000018437256,0.00028456005,0.000019841646,0.0006762843],"genre_scores_gemma":[0.99867415,0.000035799294,0.00031328245,0.000007418178,0.0000026073378,0.0000022182915,0.0006533254,0.0000052804257,0.00030590736],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999398,0.000004541744,0.0000018549159,0.000022463299,0.000012125231,0.000019178397],"domain_scores_gemma":[0.9998685,0.00001085723,0.000035567347,0.000019334368,0.000014497853,0.000051271672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008042981,0.00025495392,0.00020889007,0.0011225599,0.0002872846,0.00031436392,0.00021891606,0.00018771362,0.001092062],"category_scores_gemma":[0.00014787089,0.00015828371,0.00020139167,0.0004366852,0.00020149462,0.00017373852,0.0004547698,0.00012359346,0.00024405078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015927487,0.000042363,0.9352508,0.00003049655,0.000087042026,0.00041626953,0.0004624445,0.0021990007,0.04729533,0.00020807344,0.00064970297,0.013199297],"study_design_scores_gemma":[0.0000017769753,0.000015270285,0.9974711,0.0000028450036,0.000008821436,0.00010889514,0.00006948782,0.00071858766,0.0009380077,0.000020094458,0.0006399494,0.000005164558],"about_ca_topic_score_codex":0.01289092,"about_ca_topic_score_gemma":0.03099026,"teacher_disagreement_score":0.01289092,"about_ca_system_score_codex":0.0005033152,"about_ca_system_score_gemma":0.000098435994,"threshold_uncertainty_score":0.025631785},"labels":[],"label_agreement":null},{"id":"W2937254626","doi":"10.3847/1538-4357/ab0828","title":"A New Look into Putative Duplicity and Pulsations of the Be Star β CMi*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Grantová Agentura České Republiky","keywords":"Photometry (optics); Spectral line; Orbital period; Be star; Stellar rotation; Binary star; Radial velocity; Satellite; Rotation period","score_opus":0.008150982725488504,"score_gpt":0.22633904089957899,"score_spread":0.21818805817409048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2937254626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972626,0.00021354757,0.00038476154,0.00010646543,0.000011694562,0.000003366701,0.00006333486,0.000008301343,0.0019459903],"genre_scores_gemma":[0.9984909,0.00009276792,0.0006273111,0.00007169295,0.000027609454,0.000003743167,0.00018786803,0.0000070557185,0.0004910218],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999217,0.000013219793,0.000008123332,0.000026323189,0.000012453122,0.00001821291],"domain_scores_gemma":[0.9994048,0.0001187215,0.00015302538,0.00008214624,0.000098394215,0.00014291747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003316923,0.00015595589,0.00022983496,0.0013786934,0.0005334472,0.0007362896,0.0002281468,0.00034870047,0.0020351212],"category_scores_gemma":[0.00072286325,0.00010159273,0.00009390596,0.0005982461,0.00034618165,0.00077643385,0.00055322325,0.0004091741,0.00023660526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003464573,0.00007629508,0.8821516,0.000053728847,0.000025976813,0.0012620627,0.001490137,0.000055793607,0.09353241,0.00088239,0.00031104247,0.019812008],"study_design_scores_gemma":[0.000003911405,0.000104501734,0.9913257,0.000012835821,0.000013244068,0.0016054405,0.0010674319,0.00025029987,0.002501488,0.0006272209,0.0024815765,0.000006335253],"about_ca_topic_score_codex":0.00041301144,"about_ca_topic_score_gemma":0.00074936927,"teacher_disagreement_score":0.0020351212,"about_ca_system_score_codex":0.00012653598,"about_ca_system_score_gemma":0.0000868645,"threshold_uncertainty_score":0.006808102},"labels":[],"label_agreement":null},{"id":"W2937530065","doi":"10.3847/1538-4357/ab7cc7","title":"The Surprisingly Low Carbon Mass in the Debris Disk around HD 32297","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Astronomical Observatory of Japan; European Commission; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Research, Development and Innovation Office; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Astrophysics; Physics; Debris disk; Carbon fibers; Debris; Dissociation (chemistry); Planetesimal; Atomic physics; Chemistry; Materials science; Stars; Meteorology; Solar System; Physical chemistry; Planetary system","score_opus":0.01163645011682445,"score_gpt":0.22691327503848624,"score_spread":0.21527682492166178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2937530065","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991898,0.00009270255,0.00007810425,0.000014077903,0.000002610989,0.0000015566471,0.00013684943,0.000012716313,0.0004715206],"genre_scores_gemma":[0.9995584,0.000024840192,0.00009600088,0.000007411679,0.0000042297547,0.0000019680413,0.00016505818,0.0000043879845,0.0001377086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999523,0.0000027839244,0.0000037774848,0.000017970264,0.000012244094,0.000010856877],"domain_scores_gemma":[0.99979526,0.000027329224,0.000075184165,0.000029548191,0.00002385783,0.000048789076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001276099,0.00020138438,0.00031135377,0.00063920027,0.00045884468,0.0006249815,0.0004755294,0.00055492745,0.0010390967],"category_scores_gemma":[0.00027031728,0.00018981368,0.00018128529,0.00033231967,0.00031761263,0.00030769408,0.00033615433,0.00020110633,0.0004669974],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045236625,0.0000963508,0.75121295,0.00012322856,0.00012637106,0.0036665173,0.0006755691,0.001598037,0.23286964,0.0004730618,0.00072012236,0.007985763],"study_design_scores_gemma":[0.000024205247,0.00010335873,0.98581886,0.000015639607,0.0000454642,0.00084356527,0.00037379705,0.0035934085,0.0075903614,0.0002363891,0.0013405817,0.0000143939415],"about_ca_topic_score_codex":0.0017498003,"about_ca_topic_score_gemma":0.0018832558,"teacher_disagreement_score":0.0017498003,"about_ca_system_score_codex":0.00032795116,"about_ca_system_score_gemma":0.00010433344,"threshold_uncertainty_score":0.0034792423},"labels":[],"label_agreement":null},{"id":"W2939162290","doi":"10.3847/1538-4357/ab18a7","title":"The First Two Thousand Years of Star Formation","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Protostar; Angular momentum; Accretion (finance); Star formation; Gravitational collapse; Outflow; Magnetic field; Magnetohydrodynamics","score_opus":0.0069108348120678915,"score_gpt":0.22966691199033132,"score_spread":0.22275607717826343,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2939162290","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9693217,0.0010216067,0.008524723,0.00031999956,0.00013782055,0.000044144545,0.0025059378,0.0003011618,0.01782287],"genre_scores_gemma":[0.99327034,0.00044659257,0.0012871603,0.00009155234,0.00002109597,0.00006191711,0.0022583895,0.000068908455,0.0024939966],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988544,0.000019021187,0.0000067489714,0.000027972694,0.000021843656,0.000038953785],"domain_scores_gemma":[0.99972147,0.00007508532,0.00004483609,0.000035253048,0.00004791311,0.0000754091],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002954984,0.00032592486,0.000399444,0.00037144634,0.00062536664,0.0007074451,0.0006508019,0.00086512865,0.0055330973],"category_scores_gemma":[0.0013470607,0.0002805106,0.00081255904,0.0005584251,0.0003854882,0.0007532914,0.0005016642,0.0007106677,0.0006277676],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030894866,0.00016861415,0.08228534,0.00029639702,0.0004412981,0.0008955128,0.00028243643,0.87803686,0.0037374722,0.015046377,0.0037076403,0.0147930095],"study_design_scores_gemma":[0.00034224257,0.00040708913,0.1223274,0.0001680857,0.00027115433,0.00079090067,0.00043312574,0.8355581,0.0033741521,0.010539371,0.025656372,0.00013197438],"about_ca_topic_score_codex":0.013322917,"about_ca_topic_score_gemma":0.008930612,"teacher_disagreement_score":0.013322917,"about_ca_system_score_codex":0.00081353134,"about_ca_system_score_gemma":0.00063007284,"threshold_uncertainty_score":0.026490748},"labels":[],"label_agreement":null},{"id":"W2939489201","doi":"10.3847/1538-4357/ab12d9","title":"The ACS Fornax Cluster Survey. III. Globular Cluster Specific Frequencies of Early-type Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Galaxy; Astronomy; Galaxy cluster; Stellar mass; Virgo Cluster; Luminosity; Elliptical galaxy; Fornax Cluster; Star cluster; Star formation","score_opus":0.011029037639259146,"score_gpt":0.21350956290644232,"score_spread":0.2024805252671832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2939489201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9173027,0.0006561611,0.0003413226,0.00012878602,0.000018486871,0.00004653458,0.075143054,0.00016898684,0.0061939457],"genre_scores_gemma":[0.91973966,0.00029646434,0.0009637551,0.000091013186,0.00003945487,0.00005832921,0.07569822,0.000053005013,0.0030601418],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996711,0.000034374505,0.000023126202,0.000115836076,0.00009388362,0.0000616674],"domain_scores_gemma":[0.998899,0.00008919366,0.00044776246,0.00013624218,0.00019956543,0.0002282293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005484769,0.0002632027,0.00025621106,0.0029255536,0.00027566598,0.00043942346,0.00037974276,0.00028761209,0.0025829475],"category_scores_gemma":[0.00092948764,0.00013387292,0.00035656235,0.002330396,0.00013362091,0.00031912568,0.00048020406,0.00020922095,0.001443303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000671061,0.00002077847,0.98576874,0.000037540864,0.00008761739,0.000026159454,0.000108150525,0.00019066643,0.001313345,0.00014582643,0.005871282,0.0063628466],"study_design_scores_gemma":[0.0000019725558,0.0000035155151,0.9992387,0.0000019838942,0.000003757961,0.000008708671,0.000016469025,0.00006837682,0.00004604528,0.0000085954,0.0006008709,0.0000010765281],"about_ca_topic_score_codex":0.03590108,"about_ca_topic_score_gemma":0.052916653,"teacher_disagreement_score":0.03590108,"about_ca_system_score_codex":0.0004669967,"about_ca_system_score_gemma":0.00021866488,"threshold_uncertainty_score":0.07138419},"labels":[],"label_agreement":null},{"id":"W2939594777","doi":"10.3847/1538-4357/ab184e","title":"On the Detectability of Visible-wavelength Line Emission from the Local Circumgalactic and Intergalactic Medium","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Physics; Intergalactic travel; Surface brightness; Astrophysics; Redshift; Galaxy; Brightness; Halo; Emission spectrum; Narrowband; Astronomy; Spectral line; Optics","score_opus":0.007193020472688979,"score_gpt":0.20967497873690427,"score_spread":0.2024819582642153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2939594777","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967313,0.00009001246,0.001215665,0.00002363692,0.0000017720743,0.0000025243703,0.00007139366,0.000022413265,0.0018413721],"genre_scores_gemma":[0.9990177,0.000030424873,0.00070893025,0.000009743005,0.0000017209696,0.0000022018276,0.000068070505,0.0000026615198,0.00015858082],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991167,0.000019976727,0.0000015561118,0.000030063615,0.000019838157,0.000016996248],"domain_scores_gemma":[0.9995235,0.00024383535,0.000074976946,0.000053714837,0.000034658682,0.00006937269],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023350958,0.00017111328,0.00009719619,0.00038345094,0.00014072654,0.00032618723,0.00025300702,0.00021044779,0.0013654389],"category_scores_gemma":[0.0006266476,0.00013784981,0.0001267536,0.00014145047,0.00033865677,0.00049169606,0.00043294564,0.00014988727,0.00009903461],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085520436,0.000118499884,0.6201042,0.000089549445,0.0001389906,0.0003193653,0.00022201614,0.007887338,0.32175878,0.004180168,0.00055158354,0.043774188],"study_design_scores_gemma":[0.00003162671,0.00013474484,0.92821443,0.000015757436,0.00007016284,0.00022000802,0.00013035232,0.024475021,0.04499966,0.00066948286,0.0010118206,0.000027011594],"about_ca_topic_score_codex":0.0014824676,"about_ca_topic_score_gemma":0.003921564,"teacher_disagreement_score":0.0014824676,"about_ca_system_score_codex":0.00031046369,"about_ca_system_score_gemma":0.00006123039,"threshold_uncertainty_score":0.004567921},"labels":[],"label_agreement":null},{"id":"W2940838964","doi":"10.3847/1538-4357/ab9197","title":"The Rise and Fall of the King: The Correlation between FO Aquarii’s Low States and the White Dwarf’s Spin-down","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"White dwarf; Accretion (finance); Intermediate polar; Photometry (optics); Ephemeris; Accretion disc; Light curve; Polar","score_opus":0.010333015458930868,"score_gpt":0.21797896399435454,"score_spread":0.20764594853542367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2940838964","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977859,0.000059726943,0.00007879154,0.00006876614,0.0000061402743,0.0000028590296,0.00023132094,0.0000063543744,0.0017600699],"genre_scores_gemma":[0.99944705,0.000020199,0.000046119138,0.000009092142,0.000009974314,0.000001609452,0.0002941535,0.0000026768325,0.00016907319],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998733,0.000012384432,0.000011253669,0.00003738666,0.000027969843,0.000037693077],"domain_scores_gemma":[0.99840707,0.00022375892,0.00066100544,0.00009575341,0.00024330207,0.00036910333],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002692244,0.00009772323,0.00013175132,0.0010057947,0.00043326663,0.00084239664,0.00019783984,0.00028153652,0.001922932],"category_scores_gemma":[0.0021550541,0.00011270019,0.00009420624,0.0006122695,0.000585269,0.00040820768,0.00067424646,0.00041233798,0.00041085386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059972353,0.000013500854,0.99551684,0.0000074181758,0.000012601941,0.000052004805,0.00032254955,0.00008588464,0.0011237008,0.00016716056,0.00028488605,0.0023534591],"study_design_scores_gemma":[4.8030535e-7,0.0000073797487,0.99945146,0.0000018950791,0.0000014859221,0.000020411517,0.00013620903,0.00008247223,0.0000504121,0.000033726414,0.00021273286,0.0000012708892],"about_ca_topic_score_codex":0.007260151,"about_ca_topic_score_gemma":0.011684846,"teacher_disagreement_score":0.007260151,"about_ca_system_score_codex":0.0003803678,"about_ca_system_score_gemma":0.00016157415,"threshold_uncertainty_score":0.014435768},"labels":[],"label_agreement":null},{"id":"W2940996187","doi":"10.3847/1538-4357/ab07bc","title":"Buried Black Hole Growth in IR-selected Mergers: New Results from Chandra","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supermassive black hole; Galaxy; Active galactic nucleus; Black hole (networking); Population; Accretion (finance); Intermediate-mass black hole; Line (geometry); Infrared","score_opus":0.0071353493327708725,"score_gpt":0.20005807812464224,"score_spread":0.19292272879187136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2940996187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980603,0.0005066697,0.00054818654,0.000023015575,0.000004194794,0.00000897249,0.000102560305,0.000046869987,0.0006994036],"genre_scores_gemma":[0.9990472,0.00011577527,0.00061345514,0.0000101629585,0.000013160088,0.0000026482248,0.00014049187,0.000010154938,0.00004684896],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996903,0.00005675587,0.000022238937,0.000081059356,0.00007507782,0.000074593656],"domain_scores_gemma":[0.99830973,0.00059629325,0.00049814803,0.00020167867,0.00012424341,0.00026986867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007995957,0.0005153116,0.00049177225,0.0013695824,0.00061452814,0.0011746907,0.000615215,0.00031286417,0.0006803199],"category_scores_gemma":[0.002059447,0.00035977914,0.0005105822,0.00081977935,0.0006753281,0.00076172134,0.0010425141,0.0005431815,0.00016639665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015000429,0.0003493368,0.9261768,0.00021145269,0.0004027145,0.0027643077,0.001546669,0.0057088174,0.035153173,0.0018538263,0.00078176835,0.023551017],"study_design_scores_gemma":[0.00007546795,0.00029721067,0.96351075,0.000042827916,0.00019024713,0.0032768045,0.00060961687,0.023080768,0.0060600834,0.0011997368,0.0015826554,0.00007383414],"about_ca_topic_score_codex":0.0025189642,"about_ca_topic_score_gemma":0.0019304804,"teacher_disagreement_score":0.0025189642,"about_ca_system_score_codex":0.00033564377,"about_ca_system_score_gemma":0.0002162119,"threshold_uncertainty_score":0.0050085783},"labels":[],"label_agreement":null},{"id":"W2942461650","doi":"10.3847/1538-4357/ab6ff8","title":"Spitzer Microlensing Parallax Reveals Two Isolated Stars in the Galactic Bulge","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Fundação para a Ciência e a Tecnologia; National Research Foundation of Korea; National Natural Science Foundation of China; European Regional Development Fund; National Research Foundation; Deutsche Forschungsgemeinschaft; Ministero dell’Istruzione, dell’Università e della Ricerca; National Science Foundation","keywords":"Gravitational microlensing; Parallax; Bulge; Stars; Microlens; Lens (geology); Star (game theory); Proper motion","score_opus":0.016088357789000588,"score_gpt":0.23861297098604708,"score_spread":0.2225246131970465,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2942461650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99901783,0.000080642625,0.00016939979,0.000014168852,0.000002566809,0.0000027424098,0.00016674121,0.000023573928,0.00052226085],"genre_scores_gemma":[0.9993992,0.00001959319,0.00011218813,0.00000926854,0.0000059752665,0.0000016604208,0.00035260833,0.000004698304,0.00009483114],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999741,0.000014497,0.000015621896,0.00008903945,0.00006927974,0.00007056422],"domain_scores_gemma":[0.99901795,0.0001331891,0.00034410722,0.00012633936,0.00012217923,0.00025627908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003607809,0.0002488545,0.00038852976,0.0026048447,0.00052385655,0.00096947525,0.00030389507,0.00031878817,0.0010735722],"category_scores_gemma":[0.0006862286,0.00017116549,0.000239186,0.0008871779,0.0004743738,0.0002930888,0.0010096085,0.0002760647,0.00035864976],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024819572,0.000058107198,0.9645974,0.000024149751,0.000091831374,0.0009912541,0.0004088116,0.00024950458,0.02266097,0.00027372834,0.00033095336,0.010065119],"study_design_scores_gemma":[0.000004163167,0.00003360417,0.996992,0.0000038997005,0.000015663978,0.0004235989,0.00008992428,0.0002978893,0.0017693806,0.000060941395,0.0003041081,0.0000047716057],"about_ca_topic_score_codex":0.0026588116,"about_ca_topic_score_gemma":0.005782716,"teacher_disagreement_score":0.0026588116,"about_ca_system_score_codex":0.00061065634,"about_ca_system_score_gemma":0.00011674744,"threshold_uncertainty_score":0.005286634},"labels":[],"label_agreement":null},{"id":"W2942679849","doi":"10.3847/1538-4357/ab4efd","title":"The Ubiquitous Imprint of Radiative Acceleration in the Mean Absorption Spectrum of Quasar Outflows","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Center for Cosmology and Astroparticle Physics, Ohio State University; Carnegie Mellon University; University of California, Santa Barbara; Office of Science; Max-Planck-Institut für Astronomie; York University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory","keywords":"Quasar; Outflow; Spectral line; Superposition principle; Absorption spectroscopy; Absorption (acoustics); Radiation pressure; Radiative transfer","score_opus":0.007756326450825279,"score_gpt":0.2186380042292998,"score_spread":0.21088167777847452,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2942679849","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979639,0.000052115687,0.00083630945,0.000008763979,0.000003315024,0.0000014130376,0.00013693543,0.00007308217,0.0009241004],"genre_scores_gemma":[0.99968004,0.000006566144,0.00017997241,0.000002287179,0.000003150476,7.156807e-7,0.00008499373,0.0000059101294,0.00003645929],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998734,0.000014853782,0.0000064106007,0.00004625353,0.00003560598,0.000023353196],"domain_scores_gemma":[0.999126,0.00021013927,0.00026610878,0.00012526981,0.00010200947,0.00017054721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001898039,0.00016040627,0.0001938265,0.0009118779,0.00016913378,0.0004540962,0.00014438083,0.00014721908,0.0015593175],"category_scores_gemma":[0.0006948678,0.00011848366,0.00018208165,0.00033072074,0.00026467253,0.00023751479,0.00038460304,0.00021756248,0.00019376591],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005510598,0.0001024628,0.6240198,0.00004646351,0.00009548033,0.00020000419,0.0002502797,0.0005689583,0.3555246,0.000513357,0.00021293767,0.017914593],"study_design_scores_gemma":[0.0000027089577,0.00006544871,0.99303895,0.0000018269951,0.000012614335,0.00012973783,0.000040062743,0.00061339745,0.005828723,0.000100069075,0.00016274786,0.0000037198365],"about_ca_topic_score_codex":0.00034503915,"about_ca_topic_score_gemma":0.00036873374,"teacher_disagreement_score":0.0015593175,"about_ca_system_score_codex":0.00007061233,"about_ca_system_score_gemma":0.00004109901,"threshold_uncertainty_score":0.0052164197},"labels":[],"label_agreement":null},{"id":"W2942711334","doi":"10.3847/1538-4357/ab1e4f","title":"Virial Ratio: Direct Evaluation from Molecular Cloud Data and the Challenges of Improving Accuracy","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Virial theorem; Molecular cloud; Kinetic energy; Gravitation; Gravitational collapse; Cloud computing; Line (geometry); Measure (data warehouse); Energy balance","score_opus":0.023998171420046916,"score_gpt":0.27573789263981613,"score_spread":0.25173972121976923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2942711334","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.12704074,0.0020756796,0.8572717,0.0020781597,0.0001725057,0.00010014818,0.0006647146,0.0023694304,0.008227017],"genre_scores_gemma":[0.75012845,0.00073569454,0.24654566,0.0002925661,0.00019831292,0.000080128186,0.0005719531,0.0007854817,0.0006616804],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9941895,0.0027830368,0.00033993603,0.0005544159,0.0018867046,0.00024644844],"domain_scores_gemma":[0.9509675,0.036168803,0.0023121699,0.007397759,0.0026506162,0.00050319603],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0143010905,0.00092294626,0.0012954089,0.002445803,0.000822745,0.0038642667,0.00252892,0.0014267769,0.0019740842],"category_scores_gemma":[0.11965377,0.0006143656,0.00054132985,0.0014075649,0.0020106693,0.0076519977,0.0039130314,0.0025391623,0.0006744817],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005136071,0.00019824758,0.045957197,0.00053691294,0.00029506919,0.00047393428,0.0006546533,0.41463852,0.018554667,0.30760652,0.004561419,0.20600925],"study_design_scores_gemma":[0.000026381049,0.00005107009,0.0035055366,0.00009729757,0.000018449235,0.00014869394,0.00007327832,0.9057706,0.008103922,0.080596186,0.0015663882,0.00004220217],"about_ca_topic_score_codex":0.003764294,"about_ca_topic_score_gemma":0.0018615004,"teacher_disagreement_score":0.0143010905,"about_ca_system_score_codex":0.0013269269,"about_ca_system_score_gemma":0.00095808867,"threshold_uncertainty_score":0.075632334},"labels":[],"label_agreement":null},{"id":"W2942773692","doi":"10.3847/1538-4357/ab1d5b","title":"SDSS J075101.42+291419.1: A Super-Eddington Accreting Quasar with Extreme X-Ray Variability","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Quasar; Accretion (finance); Active galactic nucleus; Galaxy; Accretion disc; Flux (metallurgy); Spectral line; Reverberation mapping","score_opus":0.01413050310055386,"score_gpt":0.2195166878037594,"score_spread":0.20538618470320555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2942773692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974928,0.0002644122,0.00025855377,0.00008969915,0.000021658456,0.000015056008,0.0005336152,0.00004375813,0.0012804217],"genre_scores_gemma":[0.9972113,0.00011420549,0.0004327441,0.00012096534,0.000055434914,0.000008433228,0.0015140198,0.000011779272,0.0005312495],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977905,0.00001715785,0.000018481285,0.00006227334,0.00006588872,0.000057156525],"domain_scores_gemma":[0.9994235,0.000043142936,0.00023775076,0.00003969491,0.00006609534,0.00018979347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027401987,0.00044128383,0.0005106411,0.0016482947,0.00083368697,0.0007918861,0.0004298054,0.00049458677,0.001567808],"category_scores_gemma":[0.00035230877,0.00018194855,0.00027632856,0.0010265856,0.00043320202,0.00020582462,0.0005720003,0.00033029882,0.0007794589],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020517944,0.000259988,0.9147369,0.0000837152,0.00011800873,0.02684157,0.00040448143,0.00027377263,0.040511016,0.00051077903,0.003281115,0.012773326],"study_design_scores_gemma":[0.00001728171,0.00013775968,0.97394264,0.00001558397,0.000033820976,0.018152181,0.00023845749,0.0004210749,0.0023506612,0.00015492075,0.004518071,0.00001757483],"about_ca_topic_score_codex":0.0016115967,"about_ca_topic_score_gemma":0.0026509408,"teacher_disagreement_score":0.0016482947,"about_ca_system_score_codex":0.00030571187,"about_ca_system_score_gemma":0.000158676,"threshold_uncertainty_score":0.005244851},"labels":[],"label_agreement":null},{"id":"W2942922091","doi":"10.3847/1538-4357/ab3407","title":"The Far-infrared Polarization Spectrum of <i>ρ</i> Ophiuchi A from HAWC+/SOFIA Observations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Molecular cloud; Polarization (electrochemistry); Radiative transfer; Hydrogen molecule; Polarimetry; Stars; Hydrogen","score_opus":0.009819805835388563,"score_gpt":0.2121477938922909,"score_spread":0.20232798805690236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2942922091","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970427,0.000034088705,0.0004777024,0.000020104608,0.0000044324347,0.000005041909,0.0010303848,0.000074788775,0.0013107876],"genre_scores_gemma":[0.9980724,0.000042950953,0.0006203558,0.000011998787,0.000006077669,0.0000052853734,0.0011407841,0.000015825475,0.000084332416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999281,0.000006458529,0.0000027960218,0.000022319708,0.000014852003,0.00002543641],"domain_scores_gemma":[0.99986327,0.00001915445,0.00003917664,0.000024351928,0.0000202949,0.000033735225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015964075,0.0003321331,0.0001823021,0.0005577084,0.00022239368,0.00032426917,0.00024436534,0.00019455492,0.0006784694],"category_scores_gemma":[0.00021051461,0.00019189567,0.00036584015,0.0004104068,0.00024675764,0.00014344057,0.00022112652,0.00023103457,0.00014310682],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078197574,0.00012231225,0.6341037,0.00018281864,0.00041075787,0.0012160916,0.00053046434,0.030812742,0.29753175,0.0009076556,0.0036019117,0.02979775],"study_design_scores_gemma":[0.000018281986,0.00003544647,0.984124,0.000008089744,0.00004623867,0.00010328293,0.0000602852,0.009218378,0.005570671,0.00010300455,0.0006974601,0.000014840572],"about_ca_topic_score_codex":0.010132052,"about_ca_topic_score_gemma":0.009332549,"teacher_disagreement_score":0.010132052,"about_ca_system_score_codex":0.00038967573,"about_ca_system_score_gemma":0.00016253372,"threshold_uncertainty_score":0.020146132},"labels":[],"label_agreement":null},{"id":"W2943025287","doi":"10.3847/1538-4357/ab1b14","title":"Near-infrared Variability of Low-mass Stars in IC 1396A and Tr 37","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; University of California, Los Angeles; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; California Institute of Technology; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; Stars; Luminosity; Accretion (finance); Brown dwarf; Infrared; Astronomy; Galaxy","score_opus":0.0052363904428776855,"score_gpt":0.21598188847121466,"score_spread":0.21074549802833697,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2943025287","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988268,0.000060940118,0.00006713009,0.000007609996,0.0000033256263,0.000005677489,0.0005891355,0.000010564556,0.00042872925],"genre_scores_gemma":[0.9974866,0.000030439898,0.00016423484,0.000005915299,0.000009818265,0.000006285979,0.0020646718,0.000008034769,0.00022391193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965525,0.000017162223,0.000026784,0.000106044885,0.00011644718,0.000078289966],"domain_scores_gemma":[0.9987991,0.000065022345,0.0003720116,0.00010041378,0.00026973514,0.0003938567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035758136,0.00030164703,0.00045279125,0.0023578878,0.00069249223,0.000695356,0.00041136076,0.00014504677,0.0012006715],"category_scores_gemma":[0.00069777074,0.00012226257,0.00025709515,0.0019113444,0.0003520095,0.00030755711,0.0009632821,0.00022246642,0.0004923184],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006802755,0.000030215442,0.9850943,0.000012404627,0.00004954484,0.00010356713,0.00024361648,0.00014313187,0.0095597,0.00004275099,0.00024853373,0.0044042147],"study_design_scores_gemma":[0.0000016258301,0.000013555687,0.99911314,0.0000020180037,0.000005852991,0.00005760818,0.000065468834,0.00010260184,0.00030528015,0.000010194013,0.00032076734,0.000001825961],"about_ca_topic_score_codex":0.026522158,"about_ca_topic_score_gemma":0.03541484,"teacher_disagreement_score":0.026522158,"about_ca_system_score_codex":0.0007092002,"about_ca_system_score_gemma":0.00035907896,"threshold_uncertainty_score":0.052735567},"labels":[],"label_agreement":null},{"id":"W2943059545","doi":"10.3847/1538-4357/ab064f","title":"Chandra Detection of Intracluster X-Ray Sources in Fornax","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Fornax Cluster; Globular cluster; Luminosity function; Galaxy; Virgo Cluster; Astronomy; Galaxy cluster; Luminosity; Intracluster medium; Point source; Halo","score_opus":0.004400515571514535,"score_gpt":0.1897980478227433,"score_spread":0.18539753225122876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2943059545","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907994,0.00014847453,0.00009729271,0.000012965521,0.0000020897166,0.0000050356293,0.00016128844,0.000015588983,0.00047720008],"genre_scores_gemma":[0.99898165,0.00006918799,0.00037381277,0.00000856056,0.00001261238,0.000004945795,0.00039162897,0.000005719375,0.00015184813],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975306,0.000022375896,0.000016508991,0.00008380409,0.000067954956,0.00005622757],"domain_scores_gemma":[0.9989467,0.00015650035,0.0004169854,0.00015649007,0.00011068914,0.00021246934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033657285,0.0003117075,0.00036067583,0.0015165602,0.00049428677,0.00089779514,0.000399571,0.00029274085,0.0011717371],"category_scores_gemma":[0.00076217327,0.00017667301,0.00023152232,0.00089028577,0.00032351236,0.00043219907,0.00089909934,0.00024119762,0.0002925843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017949735,0.000049856688,0.9697593,0.00004477516,0.00007823842,0.00037289763,0.00037661573,0.00012437475,0.018148895,0.00024003281,0.00023057942,0.010394887],"study_design_scores_gemma":[0.000004612139,0.000028627031,0.99844354,0.0000052776913,0.000017024351,0.00030715793,0.000057543606,0.00013192782,0.0005934723,0.00004851465,0.00035919613,0.000003162536],"about_ca_topic_score_codex":0.0024207698,"about_ca_topic_score_gemma":0.0029139982,"teacher_disagreement_score":0.0024207698,"about_ca_system_score_codex":0.00023465879,"about_ca_system_score_gemma":0.00021362587,"threshold_uncertainty_score":0.004813373},"labels":[],"label_agreement":null},{"id":"W2943646757","doi":"10.3847/1538-4357/ab32dd","title":"The Delay Times of Type Ia Supernova","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto","funders":"","keywords":"Supernova; Galaxy; Luminosity; Star formation; Normalization (sociology); Type (biology); Hubble's law; Distribution (mathematics)","score_opus":0.007689150508244114,"score_gpt":0.23227390269099243,"score_spread":0.22458475218274832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2943646757","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962316,0.00011656637,0.0013811829,0.000010894237,0.000004312604,0.0000034339726,0.00076998695,0.00004916638,0.0014328477],"genre_scores_gemma":[0.99838006,0.000038704948,0.0002889558,0.0000031597424,0.0000037969521,0.000002919671,0.0008468039,0.0000107708265,0.00042475294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998827,0.000013656005,0.000009512929,0.00005040457,0.000022208373,0.000021547785],"domain_scores_gemma":[0.9975896,0.00095200137,0.0005464408,0.00022278415,0.00042292933,0.00026633986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005238308,0.00013514294,0.00013142472,0.0013679386,0.000112095484,0.0005616977,0.00020316005,0.00016250892,0.0020075229],"category_scores_gemma":[0.0030548945,0.00011386781,0.00011453316,0.0005963521,0.00017985763,0.00034237406,0.00017928524,0.00016709289,0.00036437425],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041966306,0.00003120553,0.9394157,0.000040825405,0.00008479016,0.0001292749,0.00016715682,0.006070053,0.03613724,0.003282017,0.0005588652,0.0136632025],"study_design_scores_gemma":[0.000013058979,0.00012603636,0.9682161,0.000008519467,0.0000242744,0.0004908961,0.00011818789,0.013187989,0.01365697,0.001744133,0.002395375,0.000018507084],"about_ca_topic_score_codex":0.0015252264,"about_ca_topic_score_gemma":0.0013796253,"teacher_disagreement_score":0.0020075229,"about_ca_system_score_codex":0.0003909889,"about_ca_system_score_gemma":0.000097733944,"threshold_uncertainty_score":0.0067157745},"labels":[],"label_agreement":null},{"id":"W2944065958","doi":"10.3847/1538-4357/ab3291","title":"The Lanthanide Fraction Distribution in Metal-poor Stars: A Test of Neutron Star Mergers as the Dominant r-process Site","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Kilonova; Neutron star; Ejecta; r-process; Lanthanide; Stars","score_opus":0.005985800396494558,"score_gpt":0.23312165433779533,"score_spread":0.22713585394130079,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2944065958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994453,0.002129951,0.0014606752,0.000044230706,0.0000050285103,0.0000043448836,0.00033718703,0.000052544652,0.0015130579],"genre_scores_gemma":[0.9977851,0.0006233697,0.0008853489,0.000023056851,0.000005202707,0.000003987768,0.00039283393,0.000023586279,0.0002574881],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995446,0.000004110531,0.000003578925,0.000017517963,0.000011489963,0.000008929723],"domain_scores_gemma":[0.9998173,0.00003513459,0.00008189114,0.00001325353,0.00002730599,0.000025118565],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018514293,0.00015496553,0.00023161287,0.00089160446,0.00015879543,0.00059941644,0.00019216648,0.0002557832,0.00046453287],"category_scores_gemma":[0.0003288936,0.00010206074,0.00027122055,0.00057156134,0.00016659066,0.0003771107,0.00035470017,0.0001305255,0.00019832334],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006226037,0.00002229472,0.8745686,0.000349087,0.00034071418,0.00051910663,0.000204224,0.008731805,0.078881405,0.0014976042,0.0005574387,0.033705223],"study_design_scores_gemma":[0.000015549018,0.00009261878,0.95729953,0.000051193747,0.00008940575,0.00060444407,0.00028751852,0.017456768,0.0184825,0.0015517792,0.0040487414,0.000020040286],"about_ca_topic_score_codex":0.0021268022,"about_ca_topic_score_gemma":0.0021890865,"teacher_disagreement_score":0.0021268022,"about_ca_system_score_codex":0.00030808157,"about_ca_system_score_gemma":0.00010112203,"threshold_uncertainty_score":0.00422889},"labels":[],"label_agreement":null},{"id":"W2944168985","doi":"10.3847/1538-4357/ab2131","title":"Census of the Local Universe (CLU) Narrowband Survey. I. Galaxy Catalogs from Preliminary Fields","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Smithsonian Astrophysical Observatory; University System of Taiwan; National Central University; Gordon and Betty Moore Foundation; Queen's University Belfast; Durham University; York University; Space Telescope Science Institute; Weizmann Institute of Science; Carnegie Mellon University; Los Alamos National Laboratory; College of Engineering, Michigan State University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Harvard University; Queen's University; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; National Science Foundation","keywords":"Galaxy; Redshift; Sky; Universe; Cosmology; Luminous infrared galaxy; Galaxy cluster; Galaxy formation and evolution; Field galaxy","score_opus":0.007415228003323265,"score_gpt":0.195838631438975,"score_spread":0.18842340343565175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2944168985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7190572,0.0013779101,0.0019597607,0.0001931592,0.000017617016,0.00064665446,0.26282504,0.0006680916,0.0132546015],"genre_scores_gemma":[0.55584323,0.0009147622,0.004224923,0.000226771,0.00006614235,0.0009234767,0.43213484,0.0001405773,0.0055252723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989458,0.00015757355,0.000098605036,0.0002182576,0.00036746895,0.00021227026],"domain_scores_gemma":[0.99320847,0.0005431607,0.0011615885,0.00096985925,0.0024275174,0.0016893762],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013859636,0.00049444154,0.00056671095,0.011431087,0.0007008283,0.0009784708,0.0007943072,0.0002952424,0.0058175987],"category_scores_gemma":[0.0038491804,0.00028516076,0.00040940373,0.007349927,0.0002908078,0.00072605355,0.0013914807,0.00027958173,0.0034475927],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031775434,0.00010664012,0.90956414,0.0003403935,0.00010553461,0.00017055724,0.00070391607,0.00062386115,0.004549479,0.0006840998,0.031241532,0.05159212],"study_design_scores_gemma":[0.000021196864,0.000051830917,0.9840708,0.00002621013,0.000017358252,0.000083681465,0.00014704114,0.00041720338,0.00055301073,0.000058636928,0.014541499,0.000011619444],"about_ca_topic_score_codex":0.060626294,"about_ca_topic_score_gemma":0.046750866,"teacher_disagreement_score":0.060626294,"about_ca_system_score_codex":0.0011422911,"about_ca_system_score_gemma":0.0012144927,"threshold_uncertainty_score":0.12054682},"labels":[],"label_agreement":null},{"id":"W2944198066","doi":"10.3847/1538-4357/ab164d","title":"Rejuvenation in z ∼ 0.8 Quiescent Galaxies in LEGA-C","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Elliptical galaxy; Galaxy formation and evolution; Population; Lenticular galaxy; Stellar mass; Redshift; Stellar population","score_opus":0.005958537841573753,"score_gpt":0.2088392090941418,"score_spread":0.20288067125256806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2944198066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991928,0.00004723882,0.00007526988,0.000012904316,9.671307e-7,0.0000016552624,0.00023297773,0.000009648125,0.00042651023],"genre_scores_gemma":[0.9989189,0.000016179149,0.000091849965,0.000010054133,0.0000015488,0.0000015461716,0.0007974722,0.0000029184398,0.00015960194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987245,0.000018730367,0.0000050374233,0.000041237297,0.000018810548,0.000043672066],"domain_scores_gemma":[0.9994535,0.000088684574,0.0002080276,0.000056140438,0.000054543427,0.00013908441],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002969047,0.00017051944,0.00014986012,0.0014216515,0.00028470735,0.0008521557,0.00032975542,0.00027358002,0.00084318523],"category_scores_gemma":[0.0009786959,0.000092879134,0.00020264872,0.0007903682,0.00033083328,0.00028992412,0.0005779325,0.00020004646,0.00023032812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014259078,0.000030881474,0.9857479,0.000010820937,0.000043929784,0.00016600016,0.00045275813,0.0006815079,0.007018457,0.0003106916,0.00017069528,0.0052236267],"study_design_scores_gemma":[0.000003509292,0.00002431424,0.9976706,0.000004138839,0.000008701848,0.000076027856,0.000114160284,0.0010731774,0.0003642383,0.00011397492,0.0005442682,0.0000029790474],"about_ca_topic_score_codex":0.009828723,"about_ca_topic_score_gemma":0.011222798,"teacher_disagreement_score":0.009828723,"about_ca_system_score_codex":0.00044953843,"about_ca_system_score_gemma":0.00010128966,"threshold_uncertainty_score":0.019542992},"labels":[],"label_agreement":null},{"id":"W2944459768","doi":"10.3847/1538-4357/ab1a3a","title":"Outflows in the Disks of Active Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Institut sur la Nutrition et les Aliments Fonctionnels","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Outflow; Luminosity; Disc; Extragalactic astronomy; Astronomy; Galactic plane; Galaxy formation and evolution","score_opus":0.007185807757760499,"score_gpt":0.21758422551179776,"score_spread":0.21039841775403725,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2944459768","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99839574,0.00020849866,0.00085179636,0.000008315041,0.0000018658782,0.0000026605196,0.00018791984,0.000023302056,0.00031976242],"genre_scores_gemma":[0.99938154,0.000056293262,0.0001820553,0.0000027623107,0.0000044400576,0.0000016838324,0.00029540432,0.0000028122722,0.00007302613],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998996,0.000021538885,0.000008013996,0.000035095756,0.000016467035,0.000019341556],"domain_scores_gemma":[0.9995264,0.00014645541,0.0001717292,0.000042274234,0.00004772688,0.00006541413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035624093,0.00038695065,0.00020896955,0.0010295468,0.00019157135,0.0008608203,0.0003684969,0.00029814316,0.00062663987],"category_scores_gemma":[0.0008493614,0.00015375184,0.00029075678,0.00050727185,0.00030995556,0.00044804194,0.00046892668,0.00011542178,0.00016566114],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014009127,0.000036897643,0.95563763,0.00006500742,0.00006851853,0.00033592933,0.00023397083,0.023883728,0.012445043,0.00089885923,0.00015938786,0.00609492],"study_design_scores_gemma":[0.00001990729,0.00007309935,0.9249054,0.000016071523,0.000036028952,0.00029408542,0.00016731473,0.07038367,0.002247355,0.0010178932,0.00082768966,0.000011542548],"about_ca_topic_score_codex":0.002642305,"about_ca_topic_score_gemma":0.0015031685,"teacher_disagreement_score":0.002642305,"about_ca_system_score_codex":0.0005255753,"about_ca_system_score_gemma":0.00009692935,"threshold_uncertainty_score":0.005253911},"labels":[],"label_agreement":null},{"id":"W2944516232","doi":"10.3847/1538-4357/ab1f66","title":"Confirmation of the Gaia DR2 Parallax Zero-point Offset Using Asteroseismology and Spectroscopy in the Kepler Field","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":168,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Nuclear Safety and Security Commission; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; University of California, Santa Barbara; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Parallax; Asteroseismology; Stars; Red giant; Offset (computer science); Red clump; Spectroscopy; Red-giant branch","score_opus":0.011462792917576561,"score_gpt":0.23833673450062487,"score_spread":0.2268739415830483,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2944516232","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9731704,0.00027744516,0.0047214753,0.00019713174,0.00007531617,0.000038027152,0.0031947952,0.0004950487,0.017830368],"genre_scores_gemma":[0.9882208,0.00006559305,0.004640489,0.00017430633,0.000030980482,0.000021025668,0.0042171697,0.0001762576,0.0024533556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993906,0.0000597098,0.00005254658,0.0002063235,0.0001821179,0.00010866618],"domain_scores_gemma":[0.9978079,0.00023788495,0.00040730572,0.00074465596,0.0005063011,0.0002960633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009868663,0.0003423313,0.00027528225,0.0017332796,0.00054231804,0.0010280507,0.00049197103,0.0004341574,0.0031929396],"category_scores_gemma":[0.0021648235,0.00019482782,0.00027130512,0.0009927994,0.00035302102,0.00046560212,0.00091301464,0.00052692415,0.0033781712],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010194455,0.00015285361,0.7110605,0.00012488237,0.0001096671,0.0010121982,0.00084508705,0.0009301615,0.23163764,0.0035078882,0.005080024,0.044519562],"study_design_scores_gemma":[0.00006741448,0.0002378829,0.913511,0.000039631763,0.00005457606,0.0010183288,0.00036118634,0.0019792567,0.058803856,0.0009123967,0.022977747,0.000036616668],"about_ca_topic_score_codex":0.0020796005,"about_ca_topic_score_gemma":0.0028750722,"teacher_disagreement_score":0.0031929396,"about_ca_system_score_codex":0.00052979524,"about_ca_system_score_gemma":0.00029738888,"threshold_uncertainty_score":0.010681391},"labels":[],"label_agreement":null},{"id":"W2944562053","doi":"10.3847/1538-4357/ab9814","title":"Hot Dust-obscured Galaxies with Excess Blue Light","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; National Research Foundation of Korea; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Queen's University Belfast; Durham University; York University; Space Telescope Science Institute; Ohio State University; National Research Foundation; Carnegie Mellon University; Los Alamos National Laboratory; College of Engineering, Michigan State University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Harvard University; Queen's University; California Institute of Technology; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Instituto Millenium; Vanderbilt University; Science Mission Directorate; Yale University; National Science Foundation","keywords":"Galaxy; Active galactic nucleus; Star formation; Photometry (optics); Emission spectrum; Spectroscopy; Quasar; Luminous infrared galaxy; Radio galaxy","score_opus":0.00874807281577261,"score_gpt":0.2001325193990743,"score_spread":0.1913844465833017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2944562053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99875414,0.00010687867,0.00019687058,0.000012795551,0.00000339569,0.000004197475,0.00018751924,0.00003618465,0.0006979591],"genre_scores_gemma":[0.99941015,0.000021039426,0.00015613607,0.000011334927,0.000008262331,0.000001401899,0.00017294509,0.0000030322196,0.00021578095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976486,0.00002172295,0.000020148946,0.00006367813,0.000045203327,0.00008448493],"domain_scores_gemma":[0.9989095,0.00008978175,0.0004755841,0.00012677847,0.00007477262,0.00032363672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021161704,0.0002892709,0.00037272173,0.0021419975,0.00040495428,0.00079119107,0.00033651973,0.00028197706,0.0023532899],"category_scores_gemma":[0.00040300717,0.0001808923,0.00029114183,0.0010581153,0.00039548977,0.0003069007,0.0005577232,0.0002352605,0.0004507629],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000116804455,0.00005738227,0.98277664,0.000016166747,0.000050884977,0.00045719303,0.00014597607,0.00010838858,0.012818458,0.000100607656,0.0001957385,0.0031557304],"study_design_scores_gemma":[0.000002260504,0.000037191494,0.99772435,0.0000016830903,0.000009821635,0.0007586016,0.000066653694,0.0001412941,0.00093122234,0.000046023448,0.0002786969,0.0000023140617],"about_ca_topic_score_codex":0.0016709929,"about_ca_topic_score_gemma":0.0019784141,"teacher_disagreement_score":0.0023532899,"about_ca_system_score_codex":0.00015575362,"about_ca_system_score_gemma":0.00007342514,"threshold_uncertainty_score":0.007872522},"labels":[],"label_agreement":null},{"id":"W2945098182","doi":"10.3847/1538-4357/ab1f82","title":"A New Generation of Cool White Dwarf Atmosphere Models. IV. Revisiting the Spectral Evolution of Cool White Dwarfs","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Astrophysics; Physics; Brown dwarf; Stellar classification; Atmosphere (unit); Accretion (finance); Stars; Astronomy; Meteorology","score_opus":0.013023099312007654,"score_gpt":0.21470923464609612,"score_spread":0.20168613533408847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945098182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.69036824,0.00096366525,0.2961892,0.00057187426,0.00012877274,0.000070665075,0.0015807672,0.0015520497,0.008574752],"genre_scores_gemma":[0.9403037,0.00039582932,0.0544133,0.0001546136,0.00010958321,0.000077612814,0.0011950332,0.00035374385,0.0029965416],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986696,0.000044070544,0.000009227606,0.00003691792,0.000024092284,0.00001882735],"domain_scores_gemma":[0.99962986,0.00012757615,0.00005034398,0.00008422383,0.00006027943,0.000047682544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056966895,0.0006571367,0.00056606665,0.00042261442,0.00039486613,0.0009682144,0.00086957455,0.000499591,0.0007469972],"category_scores_gemma":[0.0013038912,0.0003868743,0.00093551236,0.00031148948,0.0003028417,0.00094175455,0.0008849372,0.00061038986,0.0002707906],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009512128,0.00006451117,0.014847097,0.000044889068,0.00015256177,0.00009387529,0.00012744362,0.9497908,0.007961127,0.007984159,0.0009571025,0.017881345],"study_design_scores_gemma":[0.000014155913,0.000011449659,0.0010397863,0.0000030493968,0.000017615086,0.000012313988,0.000007833147,0.99438876,0.00038097677,0.0029029464,0.0012147167,0.0000062632184],"about_ca_topic_score_codex":0.008150372,"about_ca_topic_score_gemma":0.006694078,"teacher_disagreement_score":0.008150372,"about_ca_system_score_codex":0.00042272825,"about_ca_system_score_gemma":0.00040736338,"threshold_uncertainty_score":0.016205847},"labels":[],"label_agreement":null},{"id":"W2945719758","doi":"10.3847/1538-4357/ab223a","title":"CO Emission in Infrared-selected Active Galactic Nuclei","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Active galactic nucleus; Galaxy; Luminosity; Star formation; Luminous infrared galaxy; Infrared; Interstellar medium; Emission spectrum","score_opus":0.005042884701638012,"score_gpt":0.21464403968567297,"score_spread":0.20960115498403495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945719758","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99742174,0.00081568235,0.00021526108,0.000011525398,0.0000031127165,0.0000030093565,0.0007623579,0.000015368934,0.0007519013],"genre_scores_gemma":[0.9986247,0.00015677132,0.00016068813,0.000011072603,0.0000068904756,0.0000026255982,0.0008676213,0.000007680982,0.00016202584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971014,0.000044803783,0.000022275675,0.00011873705,0.0000655532,0.00003847578],"domain_scores_gemma":[0.9988085,0.00028171568,0.00046417923,0.00014701918,0.00019294902,0.00010567693],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005449101,0.0002428857,0.00040468454,0.003630399,0.00018364776,0.0006727749,0.0004012907,0.00021914074,0.0012633469],"category_scores_gemma":[0.0013429207,0.00012498055,0.00036568986,0.0019705542,0.00022527002,0.00032995857,0.00036155232,0.00016006433,0.00034513968],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014612573,0.000022159167,0.9812432,0.00005387362,0.00048836303,0.00007691089,0.00008258097,0.00019870844,0.011700789,0.000047075973,0.0001272298,0.005812927],"study_design_scores_gemma":[0.0000018632937,0.000026408634,0.9979546,0.000008545253,0.00012460281,0.00011229916,0.00006656843,0.00024247527,0.0011881647,0.000025305593,0.00024682397,0.0000021670498],"about_ca_topic_score_codex":0.0049296115,"about_ca_topic_score_gemma":0.0071762125,"teacher_disagreement_score":0.0049296115,"about_ca_system_score_codex":0.00028622412,"about_ca_system_score_gemma":0.00010567698,"threshold_uncertainty_score":0.009801805},"labels":[],"label_agreement":null},{"id":"W2945852308","doi":"10.3847/1538-4357/ab418c","title":"Supernova Photometric Classification Pipelines Trained on Spectroscopically Classified Supernovae from the Pan-STARRS1 Medium-deep Survey","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Supernova; Light curve; Large Synoptic Survey Telescope; Artificial intelligence; Artificial neural network; Computer science; Physics; Type (biology); Pipeline transport; Astrophysics; Algorithm; Telescope; Environmental science; Geology","score_opus":0.026983729143917227,"score_gpt":0.2555744477295067,"score_spread":0.2285907185855895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945852308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91919094,0.00022225513,0.056228273,0.00042436726,0.000067617795,0.00025025354,0.0042177965,0.01505152,0.004346961],"genre_scores_gemma":[0.9397385,0.00008704463,0.043948546,0.00020403248,0.00003178595,0.00016936597,0.0125211,0.00034230002,0.00295728],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995103,0.000062626656,0.000032923337,0.00018312778,0.00010246218,0.00010864313],"domain_scores_gemma":[0.99843854,0.00041650346,0.00014782243,0.00041154565,0.00041515593,0.00017048563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022079926,0.0009487646,0.000456914,0.0013775922,0.0005371937,0.0007215232,0.0011670308,0.0006867593,0.002608966],"category_scores_gemma":[0.0046971347,0.00045498312,0.0012267418,0.0006145999,0.0004000497,0.0011323188,0.0013892204,0.0011394074,0.0019108016],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076138624,0.00052034104,0.38947025,0.00013733793,0.00048420957,0.00014606309,0.00029541846,0.2752431,0.014561806,0.0014983829,0.01746547,0.2994162],"study_design_scores_gemma":[0.000038937706,0.00013290528,0.05731442,0.000024097326,0.000041341274,0.00006750249,0.00007010151,0.9299617,0.008327504,0.0012042759,0.0027834638,0.000033810735],"about_ca_topic_score_codex":0.017747525,"about_ca_topic_score_gemma":0.018599868,"teacher_disagreement_score":0.017747525,"about_ca_system_score_codex":0.0011974592,"about_ca_system_score_gemma":0.0012217904,"threshold_uncertainty_score":0.035288453},"labels":[],"label_agreement":null},{"id":"W2945899176","doi":"10.3847/1538-4357/ab22b9","title":"Resolved Molecular Gas and Star Formation Properties of the Strongly Lensed <i>z</i> = 2.26 Galaxy SDSS J0901+1814","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Star formation; Galaxy; Star (game theory)","score_opus":0.007031992163893441,"score_gpt":0.18161429485178698,"score_spread":0.17458230268789354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945899176","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989968,0.000038216996,0.000097451564,0.000016563423,0.0000015615232,0.0000018082109,0.0003184766,0.000020124618,0.0005090009],"genre_scores_gemma":[0.99792945,0.00004635428,0.00031197025,0.000022272248,0.000005253572,0.000004052652,0.0014709114,0.0000067745505,0.00020299788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999156,0.000005991607,0.0000056058375,0.000030154182,0.000016651004,0.000025924617],"domain_scores_gemma":[0.99982077,0.000016574919,0.00006093837,0.00001801759,0.000022374552,0.00006140308],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012615106,0.00021256323,0.00019530879,0.0008338292,0.00021809376,0.00037416889,0.0003046464,0.00021262586,0.0008445675],"category_scores_gemma":[0.00027149584,0.00018123032,0.00018282556,0.0004213933,0.00020698593,0.00023186077,0.00033438025,0.00019530358,0.0002384319],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034726763,0.00013320427,0.82921916,0.000039772513,0.00008953486,0.00035703025,0.0001958725,0.002929448,0.15909037,0.00064158253,0.0010084945,0.005948345],"study_design_scores_gemma":[0.000020281339,0.00004773992,0.9917191,0.0000034216994,0.000026628393,0.00015322091,0.0000697482,0.0031421748,0.0039931224,0.00007899008,0.00073583075,0.000009795627],"about_ca_topic_score_codex":0.007551839,"about_ca_topic_score_gemma":0.010007861,"teacher_disagreement_score":0.007551839,"about_ca_system_score_codex":0.00051780354,"about_ca_system_score_gemma":0.000117763906,"threshold_uncertainty_score":0.015015781},"labels":[],"label_agreement":null},{"id":"W2945966514","doi":"10.3847/1538-4357/ab734a","title":"Confirmation of Enhanced Long-wavelength Dust Emission in OMC 2/3","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Emissivity; Black-body radiation; Spectral line; Green Bank Telescope; Emission spectrum; Thermal emission; Spectral index; Wavelength; Telescope","score_opus":0.015034191184839386,"score_gpt":0.24493821271756783,"score_spread":0.22990402153272843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2945966514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99771523,0.00007120127,0.00040152945,0.00004516834,0.0000063374882,0.000009582417,0.00041790702,0.00005653473,0.0012765942],"genre_scores_gemma":[0.9985435,0.00001864636,0.00067403953,0.000054950033,0.000010118098,0.000008589133,0.00054965576,0.000020797925,0.000119758246],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975294,0.0000098833,0.000009637041,0.00007501539,0.000072664436,0.000079805206],"domain_scores_gemma":[0.99946314,0.000034695946,0.00018147643,0.000051940293,0.0000897168,0.00017907178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003045683,0.00037386012,0.0004187797,0.0014718826,0.0009944486,0.0008675482,0.00050228334,0.00049388857,0.0011448981],"category_scores_gemma":[0.00032391632,0.0003103595,0.00040369216,0.00085621513,0.00049211923,0.00025557575,0.00062649563,0.000689442,0.0002563963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002566797,0.00011767802,0.67981064,0.00006263598,0.000108904664,0.000957138,0.00067869894,0.0004447223,0.310977,0.00046000496,0.0008463764,0.00527943],"study_design_scores_gemma":[0.000010482214,0.000030237832,0.99308634,0.000008548646,0.000016133119,0.00026270072,0.00016287317,0.00064184715,0.004846456,0.000100036734,0.0008276322,0.0000067000688],"about_ca_topic_score_codex":0.008076991,"about_ca_topic_score_gemma":0.018104354,"teacher_disagreement_score":0.008076991,"about_ca_system_score_codex":0.0013020973,"about_ca_system_score_gemma":0.0002677492,"threshold_uncertainty_score":0.016059935},"labels":[],"label_agreement":null},{"id":"W2946216190","doi":"10.3847/1538-4357/ab2246","title":"Extreme CO Isotopologue Line Ratios in ULIRGS: Evidence for a Top-heavy IMF","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Isotopologue; Galaxy; Line (geometry); Interstellar medium; Nucleosynthesis; Star formation; Infrared; Astrochemistry; Active galactic nucleus","score_opus":0.043004927545760775,"score_gpt":0.30810943753814285,"score_spread":0.26510450999238205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2946216190","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995009,0.000028932254,0.000080989514,0.0000041407257,4.7387954e-7,9.3263264e-7,0.000034059107,0.000011531154,0.000338073],"genre_scores_gemma":[0.9998448,0.0000059720383,0.00006430694,0.0000054546285,6.6935695e-7,6.0192883e-7,0.00003249195,0.0000012557388,0.00004446806],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999913,0.000010040527,0.0000050786925,0.000024342085,0.000017838085,0.000029644256],"domain_scores_gemma":[0.99966335,0.000033086777,0.0001265859,0.000037742204,0.00004708458,0.00009220797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015840253,0.00015631945,0.00019485234,0.00089197414,0.00025500398,0.00045285167,0.00020901138,0.00018405815,0.0007696945],"category_scores_gemma":[0.0003114583,0.000109751534,0.00009764973,0.00033837196,0.0004121444,0.00014055583,0.00027991808,0.00016742974,0.00016883232],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018215587,0.000027987626,0.92668384,0.000010010674,0.000033033353,0.00036599248,0.0002718402,0.00012421099,0.06861691,0.00010801769,0.00006497012,0.003511066],"study_design_scores_gemma":[0.000001913969,0.00003091309,0.99626946,0.0000017938968,0.000008801352,0.00023625372,0.00017347677,0.00018734374,0.0029362643,0.000033702727,0.000117880125,0.0000020934374],"about_ca_topic_score_codex":0.0031436353,"about_ca_topic_score_gemma":0.0048330068,"teacher_disagreement_score":0.0031436353,"about_ca_system_score_codex":0.00024449095,"about_ca_system_score_gemma":0.00005153423,"threshold_uncertainty_score":0.0062506795},"labels":[],"label_agreement":null},{"id":"W2946594096","doi":"10.3847/1538-4357/ab1f77","title":"Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"National Institutes of Natural Sciences; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Research Foundation; Danmarks Grundforskningsfond; National Astronomical Observatory of Japan; European Commission; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Narodowym Centrum Nauki; National Science Foundation","keywords":"Galaxy; Spiral galaxy; Star formation; Redshift; Stellar mass; Stellar population; Mass ratio; Population","score_opus":0.006975862788868328,"score_gpt":0.2016635041799516,"score_spread":0.19468764139108327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2946594096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987741,0.00006845533,0.00028322445,0.000009716182,0.0000017721367,0.0000025911486,0.00031715402,0.00004328031,0.00049956416],"genre_scores_gemma":[0.9988901,0.000016543596,0.00041027175,0.000008071367,0.0000068725444,0.0000023563439,0.0005562892,0.000005480608,0.00010392519],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986494,0.000014785945,0.0000075606267,0.00004456996,0.000031985186,0.0000362364],"domain_scores_gemma":[0.999345,0.00008248774,0.0002414719,0.00007723626,0.00009784748,0.00015595178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004250683,0.00027825797,0.0002707937,0.002489944,0.00019493727,0.0006807243,0.00027652385,0.0002607989,0.0010249951],"category_scores_gemma":[0.0005532061,0.00019408617,0.0002649932,0.00093760446,0.00014881209,0.00029317348,0.00054947316,0.00015375667,0.0004140887],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052134772,0.000022602886,0.98175186,0.000010669865,0.000042618412,0.00004327589,0.00011983663,0.00026842402,0.013035408,0.000090947105,0.00011348858,0.004448761],"study_design_scores_gemma":[0.0000019458896,0.000011647391,0.9989625,0.0000012303802,0.000005767878,0.000030820465,0.000025956828,0.00038906775,0.00041900727,0.00002372637,0.00012697431,0.0000013510146],"about_ca_topic_score_codex":0.00297675,"about_ca_topic_score_gemma":0.005493566,"teacher_disagreement_score":0.00297675,"about_ca_system_score_codex":0.0002921634,"about_ca_system_score_gemma":0.00008767305,"threshold_uncertainty_score":0.0059188604},"labels":[],"label_agreement":null},{"id":"W2946929753","doi":"10.3847/1538-4357/ab6e64","title":"Wide-band Rotation Measure Synthesis","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Faraday effect; Measure (data warehouse); Interferometry; Polarimetry; Rotation (mathematics); Fourier transform; Faraday cage; Range (aeronautics)","score_opus":0.019002115582126465,"score_gpt":0.2879419044908958,"score_spread":0.26893978890876935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2946929753","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.10697192,0.00017119235,0.88225126,0.00018532261,0.0001065572,0.00004972251,0.0004952639,0.0009531756,0.008815573],"genre_scores_gemma":[0.7831579,0.000108618544,0.21347556,0.00008235633,0.00004537309,0.00008349608,0.0008460064,0.00019256835,0.002008042],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99968433,0.00006803977,0.000017029697,0.00009371605,0.000087845525,0.000049001042],"domain_scores_gemma":[0.9994609,0.00017359917,0.00006734615,0.00013494374,0.00012417416,0.00003910034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005665138,0.00042706233,0.00047981195,0.00050723006,0.0002352993,0.00082181883,0.00048407997,0.0003712465,0.0035471625],"category_scores_gemma":[0.0018968786,0.00017726564,0.00040501682,0.00042644277,0.00047782244,0.0008973791,0.0008472956,0.00044906282,0.00061364006],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025584473,0.00007443785,0.0038997792,0.00014055448,0.0000813432,0.00011042564,0.00016461956,0.6875015,0.039937474,0.110158645,0.0027577097,0.15491764],"study_design_scores_gemma":[0.000020567619,0.00007253029,0.0011493347,0.00001562325,0.000012601458,0.0000657485,0.00004263413,0.94048816,0.017886411,0.034197427,0.006021035,0.000027925103],"about_ca_topic_score_codex":0.00088534923,"about_ca_topic_score_gemma":0.00075441215,"teacher_disagreement_score":0.0035471625,"about_ca_system_score_codex":0.0003787141,"about_ca_system_score_gemma":0.0003803625,"threshold_uncertainty_score":0.01186645},"labels":[],"label_agreement":null},{"id":"W2946932776","doi":"10.3847/1538-4357/ab3e6c","title":"ALMA Unveils Widespread Molecular Gas Clumps in the Ram Pressure Stripped Tail of the Norma Jellyfish Galaxy","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Nuclear Safety and Security Commission; Grantová Agentura České Republiky; Science and Technology Facilities Council; Ministério da Ciência, Tecnologia e Ensino Superior; European Commission; Fundação para a Ciência e a Tecnologia; Australian Government; National Aeronautics and Space Administration; National Science Foundation","keywords":"Galaxy; Molecular cloud; Cluster (spacecraft); Stars; Ram pressure; Intracluster medium; Barred spiral galaxy; Star formation","score_opus":0.00456320947939827,"score_gpt":0.19735016901913097,"score_spread":0.19278695953973268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2946932776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985306,0.00012512761,0.0004929808,0.000016153575,0.0000020663529,0.000002172749,0.00012630169,0.00006912609,0.0006353935],"genre_scores_gemma":[0.999183,0.000022961029,0.00043248056,0.0000120435,0.000004991813,0.0000018800345,0.00013049498,0.00000833084,0.00020383774],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992776,0.0000030697915,0.0000024650242,0.000026900523,0.000015797601,0.000023938075],"domain_scores_gemma":[0.99963367,0.000037054826,0.0001213176,0.000059568574,0.000043184948,0.000105264226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013090554,0.0002065467,0.00023675329,0.0008365175,0.00027604366,0.0005350531,0.00036556457,0.00023726285,0.00173829],"category_scores_gemma":[0.0002623899,0.00022041902,0.00021935608,0.00026718588,0.0003391215,0.0004056693,0.00065919576,0.00024697348,0.00038301837],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003312641,0.000029267721,0.35077262,0.00006196012,0.00007916435,0.0012347916,0.0003654433,0.00076087634,0.63458884,0.00019187498,0.00021944137,0.011364445],"study_design_scores_gemma":[0.000009026711,0.00008489169,0.9754013,0.00001082877,0.000029911742,0.0005671236,0.00023520632,0.003884746,0.01846332,0.00014847424,0.0011506046,0.000014645108],"about_ca_topic_score_codex":0.0015725319,"about_ca_topic_score_gemma":0.0024478016,"teacher_disagreement_score":0.00173829,"about_ca_system_score_codex":0.0002620234,"about_ca_system_score_gemma":0.00007845794,"threshold_uncertainty_score":0.0058151484},"labels":[],"label_agreement":null},{"id":"W2946952120","doi":"10.3847/1538-4357/ab3578","title":"XMM-Newton Detection and Spectrum of the Second Fastest Spinning Pulsar PSR J0952−0607","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Science and Technology Facilities Council; Russian Foundation for Basic Research; National Aeronautics and Space Administration","keywords":"Pulsar; Neutron star; Luminosity; Millisecond pulsar; Spectral line; Dimensionless quantity; Amplitude; X-ray pulsar; Binary pulsar","score_opus":0.00610333329635758,"score_gpt":0.26366973478118255,"score_spread":0.25756640148482496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2946952120","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9870433,0.00066076964,0.0010796806,0.000344131,0.00007147924,0.000032816843,0.0019436311,0.00019107688,0.008633217],"genre_scores_gemma":[0.99055976,0.0002329113,0.00387787,0.00035556857,0.0001042242,0.000034209846,0.0031548517,0.000045042078,0.0016354283],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998035,0.00001925212,0.000016258948,0.000055830133,0.000075224365,0.000030099147],"domain_scores_gemma":[0.99956566,0.000060403192,0.00011926699,0.000042646046,0.0000885441,0.00012346258],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035578152,0.00036895933,0.00034720774,0.0016220772,0.00047467032,0.00043530244,0.00031897513,0.00073734636,0.0025544455],"category_scores_gemma":[0.00037320296,0.00019787095,0.00027111737,0.0005875721,0.0002613109,0.00024171697,0.0005013857,0.00044466258,0.00093803334],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003053624,0.00021435544,0.6662403,0.00016620722,0.00018519824,0.0031296767,0.00043676616,0.0003132452,0.2843868,0.0015281434,0.0077305078,0.035363432],"study_design_scores_gemma":[0.000015605328,0.00016666634,0.985615,0.000022999417,0.000039587932,0.0021407343,0.000064436805,0.00096768443,0.0061604455,0.00012748285,0.0046671,0.000012145227],"about_ca_topic_score_codex":0.0010342633,"about_ca_topic_score_gemma":0.0022858537,"teacher_disagreement_score":0.0025544455,"about_ca_system_score_codex":0.00025459804,"about_ca_system_score_gemma":0.00011087962,"threshold_uncertainty_score":0.008545458},"labels":[],"label_agreement":null},{"id":"W2948067881","doi":"10.3847/1538-4357/ab286f","title":"JCMT BISTRO Survey Observations of the Ophiuchus Molecular Cloud: Dust Grain Alignment Properties Inferred Using a Ricean Noise Model","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Japan Society for the Promotion of Science; Science and Technology Facilities Council; National Key Research and Development Program of China; National Research Foundation of Korea","keywords":"Ophiuchus; Polarization (electrochemistry); Star formation; Magnetic field; Stokes parameters; Interstellar medium; Protostar; Cosmic dust","score_opus":0.046206028833023674,"score_gpt":0.2492844173622856,"score_spread":0.2030783885292619,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2948067881","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9793185,0.000044757086,0.019494515,0.00008833375,0.0000036684723,0.000011155335,0.00015712899,0.00011061817,0.00077149033],"genre_scores_gemma":[0.9991629,0.000014256565,0.0006359013,0.000008762349,0.000003579931,0.0000042999914,0.000064293185,0.000008428567,0.000097499185],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99987495,0.000025321593,0.0000053972876,0.000042471012,0.000024155606,0.00002771853],"domain_scores_gemma":[0.9996039,0.0001396984,0.000118622134,0.00005433155,0.000043014235,0.00004049239],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047697168,0.00042511473,0.00022528377,0.0004104952,0.00023523493,0.00061238324,0.00054470083,0.00047776892,0.00027124461],"category_scores_gemma":[0.0016692072,0.0002344812,0.00034647633,0.00025995905,0.00045984125,0.00054026826,0.00022796242,0.00021540119,0.000072206814],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036168337,0.00007257642,0.22571279,0.000047975474,0.00014773753,0.00037101455,0.00015633373,0.7154765,0.039264645,0.0090536075,0.00078740355,0.008547719],"study_design_scores_gemma":[0.0000114585455,0.000016960312,0.043307345,0.0000030988726,0.000009284334,0.00003730449,0.000014982004,0.9543368,0.0011489496,0.0010090845,0.00009646987,0.00000831636],"about_ca_topic_score_codex":0.015022663,"about_ca_topic_score_gemma":0.007823876,"teacher_disagreement_score":0.015022663,"about_ca_system_score_codex":0.0010954995,"about_ca_system_score_gemma":0.00029426336,"threshold_uncertainty_score":0.02987045},"labels":[],"label_agreement":null},{"id":"W2948436616","doi":"10.3847/1538-4357/ab2713","title":"First Determination of 2D Speed Distribution within the Bodies of Coronal Mass Ejections with Cross-correlation Analysis","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Coronal mass ejection; Orbiter; Physics; Observatory; Interplanetary spaceflight; Solar observatory; Doppler effect; Astrophysics; Astronomy; Solar wind; Plasma","score_opus":0.0049560577706308,"score_gpt":0.22907855374986108,"score_spread":0.22412249597923029,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2948436616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8291641,0.0002449547,0.16664581,0.000040710114,0.00003704606,0.000055801534,0.0010599631,0.0008242942,0.0019273502],"genre_scores_gemma":[0.9443922,0.00016326037,0.05315046,0.000014557732,0.00003390816,0.000038279202,0.0015337403,0.000079687794,0.00059395604],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.999828,0.000020863165,0.000008919317,0.000051133604,0.00005267788,0.000038395046],"domain_scores_gemma":[0.99922764,0.00014909389,0.00014096701,0.00007931936,0.00033266156,0.00007029612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028808467,0.00042879034,0.00024658782,0.0033681714,0.00022516072,0.000567887,0.0002438333,0.00027763733,0.0010969626],"category_scores_gemma":[0.0009715432,0.00018779474,0.0003313775,0.0016488691,0.00015881921,0.0003555245,0.00036313923,0.00023613717,0.00035163818],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058757106,0.00034716388,0.23093006,0.00026265153,0.00030365973,0.0015478473,0.0005463045,0.104640126,0.29685026,0.0029230046,0.0039078705,0.35715348],"study_design_scores_gemma":[0.0000095169335,0.00009456395,0.2507392,0.000017670653,0.00005824293,0.0005406165,0.0001143663,0.71567255,0.03026635,0.00040782473,0.0020281079,0.000051033127],"about_ca_topic_score_codex":0.0033183943,"about_ca_topic_score_gemma":0.0037931546,"teacher_disagreement_score":0.0033681714,"about_ca_system_score_codex":0.00021493959,"about_ca_system_score_gemma":0.00028300023,"threshold_uncertainty_score":0.0065981746},"labels":[],"label_agreement":null},{"id":"W2948963662","doi":"10.3847/1538-4357/ab7ffb","title":"Finding Strong Gravitational Lenses in the DESI DECam Legacy Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":96,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Perimeter Institute","funders":"","keywords":"Physics; Astronomy; Gravitational lens; Gravitation; Astrophysics; Galaxy","score_opus":0.04710150571412908,"score_gpt":0.2774717757781088,"score_spread":0.2303702700639797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2948963662","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99535406,0.00010458651,0.00055216916,0.000038469945,0.0000045013835,0.000012167559,0.0021007264,0.00021182274,0.0016215973],"genre_scores_gemma":[0.98901653,0.00006262443,0.0031477294,0.000029768185,0.000010922483,0.0000060335788,0.0067705736,0.00003590023,0.0009198596],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980885,0.000022255366,0.000010500146,0.000055361892,0.00006131838,0.00004183022],"domain_scores_gemma":[0.9993875,0.0001044285,0.00013375563,0.000091691705,0.00011872761,0.00016377225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000393382,0.00028614825,0.00020838398,0.0016341483,0.0002793675,0.0005226997,0.00021995883,0.00013682379,0.0014424106],"category_scores_gemma":[0.00075467955,0.0001334531,0.00020643607,0.0008254093,0.00015447233,0.00016615662,0.0006434495,0.0001502933,0.0005956662],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002997684,0.00008372691,0.927059,0.00006564353,0.00014120653,0.00028024748,0.00024536156,0.0026930212,0.014393652,0.00018139146,0.0040949946,0.0504621],"study_design_scores_gemma":[0.000011384397,0.000041945113,0.9896142,0.0000086882665,0.000024032925,0.00013140145,0.00017637908,0.0048953625,0.0027722137,0.000073177725,0.002243908,0.000007393747],"about_ca_topic_score_codex":0.009715466,"about_ca_topic_score_gemma":0.036347616,"teacher_disagreement_score":0.009715466,"about_ca_system_score_codex":0.0002913206,"about_ca_system_score_gemma":0.00022699728,"threshold_uncertainty_score":0.019317806},"labels":[],"label_agreement":null},{"id":"W2949157900","doi":"10.3847/1538-4357/ab2909","title":"Toward a Full MHD Jet Model of Spinning Black Holes. I. Framework and a Split Monopole Example","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Magnetohydrodynamics; Bernoulli's principle; Classical mechanics; Mechanics; Magnetic field; Jet (fluid); Plasma; Magnetic monopole; Equations of motion; Quantum mechanics","score_opus":0.029948395697461678,"score_gpt":0.24406419049782135,"score_spread":0.21411579480035967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949157900","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.40438673,0.0033341087,0.5015739,0.004451978,0.00059679814,0.00021169602,0.0004228588,0.0004469027,0.08457507],"genre_scores_gemma":[0.93693805,0.0008908132,0.047925424,0.0005063734,0.00041109763,0.0001778418,0.000136787,0.00012443606,0.0128890965],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998135,0.00008577798,0.000006745577,0.000018387072,0.00004592757,0.000029639103],"domain_scores_gemma":[0.99979514,0.000040297364,0.00003587846,0.000024143592,0.000034025787,0.000070610244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053711794,0.0009366933,0.0010251049,0.0007171545,0.0010324622,0.0014906661,0.0018806743,0.0024172615,0.0021420482],"category_scores_gemma":[0.000735508,0.00050842616,0.0014910685,0.0003910899,0.0021796995,0.0014808902,0.001715631,0.0011974489,0.00046815132],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000108898625,0.00011738242,0.00080107496,0.00013032439,0.000055169716,0.0006334681,0.00024145517,0.41322362,0.0074847317,0.57320845,0.0014253733,0.0025700233],"study_design_scores_gemma":[0.000047323163,0.000023620716,0.00018331851,0.000007933749,0.000005796256,0.000045636196,0.000030598105,0.9457764,0.0001276235,0.05316847,0.0005721873,0.000011270615],"about_ca_topic_score_codex":0.0054103886,"about_ca_topic_score_gemma":0.0025485998,"teacher_disagreement_score":0.0054103886,"about_ca_system_score_codex":0.0008734443,"about_ca_system_score_gemma":0.00068343425,"threshold_uncertainty_score":0.010757804},"labels":[],"label_agreement":null},{"id":"W2949209914","doi":"10.1086/318906","title":"A Monte Carlo Study of the 6.4 [CLC]ke[/CLC]V Emission at the Galactic Center","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"X-ray Spectroscopy and Fluorescence Analysis","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Galactic Center; Sagittarius A*; Astrophysics; Monte Carlo method; Line (geometry); Emission spectrum; Black hole (networking); Point source; Luminosity; Radiation; Astronomy; Spectral line; Optics; Stars; Geometry; Galaxy","score_opus":0.008258920016794579,"score_gpt":0.24945222173061468,"score_spread":0.2411933017138201,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949209914","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9819926,0.00039185333,0.009398375,0.00042393294,0.000027384966,0.000061414015,0.00064510695,0.00014868098,0.0069106063],"genre_scores_gemma":[0.98895746,0.00015162167,0.008242871,0.000100650934,0.000018119958,0.00008520557,0.00089367985,0.00004927855,0.0015010224],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996637,0.00015069872,0.000012663961,0.000040680097,0.00004337322,0.00008889411],"domain_scores_gemma":[0.98944515,0.008666171,0.00050449785,0.0002946765,0.00064813154,0.00044140941],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015845591,0.0005822029,0.00080123224,0.0007818908,0.00097148214,0.00083984155,0.0011963049,0.0014769187,0.0036676251],"category_scores_gemma":[0.0063907546,0.0006549821,0.00079517503,0.000996517,0.0010759942,0.00069443585,0.00054350356,0.00134771,0.00017865759],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024502134,0.00012967459,0.0063264645,0.00004712523,0.00008074592,0.00010965527,0.00004554672,0.9860675,0.00035843044,0.0043843337,0.0005737091,0.0016318634],"study_design_scores_gemma":[0.00006127802,0.00005378665,0.0012364914,0.0000075299213,0.000021711801,0.00002079304,0.000030906733,0.99743146,0.00016598072,0.00079641043,0.00016561626,0.000008019176],"about_ca_topic_score_codex":0.044604994,"about_ca_topic_score_gemma":0.04342393,"teacher_disagreement_score":0.044604994,"about_ca_system_score_codex":0.001610562,"about_ca_system_score_gemma":0.0016241489,"threshold_uncertainty_score":0.0886907},"labels":[],"label_agreement":null},{"id":"W2949517756","doi":"10.3847/1538-4357/ab2b98","title":"The REASONS Survey: Resolved Millimeter Observations of a Large Debris Disk around the Nearby F Star HD 170773","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Planetesimal; RADIUS; Debris disk; Exoplanet; Planetary system; Stars; Debris; Luminosity; Solar mass","score_opus":0.023497632397838163,"score_gpt":0.24302193878681388,"score_spread":0.21952430638897572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949517756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99729913,0.000055246255,0.00038893663,0.000029887511,0.0000037671025,0.000013366649,0.0011569858,0.00006366754,0.0009889789],"genre_scores_gemma":[0.996546,0.00002715598,0.0014996657,0.000034113993,0.000010746498,0.000010656598,0.0015733584,0.0000069360067,0.00029137265],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999175,0.0000068298386,0.000004017031,0.000018474184,0.000026182546,0.000026942507],"domain_scores_gemma":[0.99965155,0.00003398743,0.00011331455,0.000032314332,0.00004443886,0.000124348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002002306,0.00015317718,0.00018662447,0.0009206912,0.00037665816,0.00026443895,0.0001999801,0.0002946339,0.0010167558],"category_scores_gemma":[0.00020884603,0.00013082207,0.00020743681,0.00052271486,0.00011633947,0.00012259121,0.00023939864,0.00017697837,0.0003130059],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003152312,0.0002051911,0.884918,0.00006815815,0.00012446144,0.0008158218,0.00054782577,0.0016719897,0.071047105,0.0004299704,0.004590797,0.035265476],"study_design_scores_gemma":[0.00001823582,0.00006469557,0.9945655,0.0000032892676,0.0000156685,0.00020280929,0.00010855205,0.0019326138,0.001412138,0.00003549815,0.0016357227,0.0000052396485],"about_ca_topic_score_codex":0.014844536,"about_ca_topic_score_gemma":0.044549838,"teacher_disagreement_score":0.014844536,"about_ca_system_score_codex":0.0004374691,"about_ca_system_score_gemma":0.0003091201,"threshold_uncertainty_score":0.02951628},"labels":[],"label_agreement":null},{"id":"W2949522415","doi":"10.1086/519454","title":"The Wolf-Rayet Population Predicted by Massive Single Star and Massive Binary Evolution","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Astrophysics; Metallicity; Physics; Stars; Wolf–Rayet star; Supergiant; Binary number; Stellar evolution; Binary star; Population; Star (game theory); Astronomy; Mathematics; Medicine","score_opus":0.006599173739746931,"score_gpt":0.2109284872183124,"score_spread":0.20432931347856545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949522415","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98763883,0.0001103494,0.007857463,0.000040986895,0.0000075717917,0.000011151242,0.00006743266,0.000032947966,0.004233297],"genre_scores_gemma":[0.99788326,0.00006792839,0.0012446202,0.000011248958,0.000006839691,0.000008590808,0.00009079384,0.000009596542,0.00067717634],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988985,0.00001867273,0.000007729124,0.000040862702,0.000023703187,0.000019183915],"domain_scores_gemma":[0.9993349,0.0002521939,0.0002059489,0.00008369589,0.000042146024,0.00008104305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049482915,0.00024792165,0.000270115,0.00068363134,0.00024085314,0.0008347398,0.0005528693,0.000297146,0.0020322236],"category_scores_gemma":[0.0024725571,0.00012632838,0.00020342386,0.00024213124,0.00045569084,0.00071434554,0.00051785534,0.00023207089,0.00030996266],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037746722,0.00011091379,0.5998509,0.0001591865,0.00006528175,0.0016229516,0.00059600436,0.12235527,0.030783154,0.2013801,0.000962188,0.04173665],"study_design_scores_gemma":[0.000058467333,0.0002753978,0.28704205,0.00004539743,0.000046455785,0.0022900375,0.00024759542,0.5627207,0.0122562405,0.13188644,0.0030915402,0.000039755752],"about_ca_topic_score_codex":0.000398632,"about_ca_topic_score_gemma":0.0004075275,"teacher_disagreement_score":0.0020322236,"about_ca_system_score_codex":0.0003433136,"about_ca_system_score_gemma":0.00010816295,"threshold_uncertainty_score":0.006798446},"labels":[],"label_agreement":null},{"id":"W2949547566","doi":"10.3847/1538-4357/aaf1c6","title":"Resolving CO (2−1) in z ∼ 1.6 Gas-rich Cluster Galaxies with ALMA: Rotating Molecular Gas Disks with Possible Signatures of Gas Stripping","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto; York University","funders":"Astrophysics Division; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Council; National Institutes of Natural Sciences; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; European Southern Observatory; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy cluster; Galaxy; Cluster (spacecraft); Virgo Cluster; Star formation; Redshift; Astronomy","score_opus":0.0045292563048613425,"score_gpt":0.20727489072646024,"score_spread":0.2027456344215989,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949547566","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991273,0.00008933776,0.00023754842,0.000014422275,0.0000014692688,0.000003633508,0.000097722106,0.000035147663,0.00039340905],"genre_scores_gemma":[0.99937123,0.000013080571,0.00038322195,0.000013686742,0.0000041364387,0.000002064506,0.000116671064,0.0000037754842,0.00009204951],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998386,0.000011463066,0.0000049083046,0.00006170244,0.000028629844,0.000054778575],"domain_scores_gemma":[0.99962115,0.000049392318,0.0000953403,0.000057632686,0.00005635908,0.00012008156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027835983,0.0002713147,0.00026293207,0.0014134861,0.00042341024,0.0006479118,0.00037575423,0.0002666291,0.0009110911],"category_scores_gemma":[0.00034135216,0.00019324668,0.00017090878,0.0005250163,0.0003147745,0.00026955316,0.00057615247,0.00017211602,0.00027829298],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032571406,0.00005793822,0.8682989,0.000021907828,0.00008687071,0.00023212738,0.00039192347,0.00039768004,0.12025421,0.00014366346,0.0002972762,0.009491769],"study_design_scores_gemma":[0.0000061002784,0.00004710279,0.99531835,0.0000025615266,0.000022883782,0.00014751768,0.00014302242,0.0007409959,0.0031619247,0.00005676606,0.0003481834,0.0000046170094],"about_ca_topic_score_codex":0.0045794602,"about_ca_topic_score_gemma":0.009850568,"teacher_disagreement_score":0.0045794602,"about_ca_system_score_codex":0.00035431725,"about_ca_system_score_gemma":0.000096556745,"threshold_uncertainty_score":0.009105623},"labels":[],"label_agreement":null},{"id":"W2949557391","doi":"10.1086/374657","title":"Saturation of the<i>r</i>‐Mode Instability","year":2003,"lang":"zh","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":230,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Saturation (graph theory); Gravitational wave; Instability; Neutron star; Amplitude; Stars; Stellar pulsation; Inertial frame of reference","score_opus":0.012698608713206725,"score_gpt":0.30945194391717246,"score_spread":0.29675333520396574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949557391","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9808444,0.00008554121,0.0072397618,0.00006357591,0.0000056980684,0.000017034588,0.000018147963,0.000093621544,0.011632106],"genre_scores_gemma":[0.9991543,0.00003156247,0.0003995694,0.0000066428615,0.0000015513117,0.00000607165,0.000007808512,0.000013264739,0.0003792246],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.999944,0.000011871789,0.00000230993,0.000005877578,0.000014949866,0.000021065807],"domain_scores_gemma":[0.9998313,0.00007643093,0.000030679632,0.000018349547,0.000021591213,0.00002163526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014353334,0.00023948631,0.00016667311,0.00020525785,0.00021423513,0.00031045004,0.00023451608,0.0002075286,0.0016310822],"category_scores_gemma":[0.0008234634,0.00014523041,0.000292538,0.00007637343,0.00047790215,0.0004794268,0.00056750985,0.00033788505,0.0002470724],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005861995,0.0001938903,0.04051484,0.00039317214,0.00007886393,0.0011996512,0.0012219573,0.31002903,0.5474141,0.064217135,0.0009628553,0.03318823],"study_design_scores_gemma":[0.00003353465,0.000114401904,0.010079858,0.000016693619,0.000010235931,0.00014585833,0.000098184886,0.92519337,0.056687117,0.0069050416,0.0007005661,0.000015151461],"about_ca_topic_score_codex":0.0011013751,"about_ca_topic_score_gemma":0.0003289648,"teacher_disagreement_score":0.0016310822,"about_ca_system_score_codex":0.00023502197,"about_ca_system_score_gemma":0.00026310282,"threshold_uncertainty_score":0.005456507},"labels":[],"label_agreement":null},{"id":"W2949573098","doi":"10.3847/1538-4357/ab2f72","title":"The HERA-19 Commissioning Array: Direction-dependent Effects","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McGill University","funders":"Science and Technology Facilities Council; Australian Research Council; Royal Society","keywords":"Reionization; Polarization (electrochemistry); Sky; Polarimetry; Astronomical interferometer; Radiative transfer; Interferometry; Stokes parameters; Spectral density","score_opus":0.0047764058617610445,"score_gpt":0.21754915727896215,"score_spread":0.21277275141720112,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949573098","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9646171,0.0002532905,0.02647857,0.00016865095,0.000031714215,0.000020768164,0.0007803902,0.0006941457,0.0069554793],"genre_scores_gemma":[0.99546707,0.000042815558,0.0035763113,0.000048035366,0.000009317304,0.000005249943,0.00041356368,0.00012583462,0.00031174166],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9992274,0.00020489127,0.000024978559,0.0001723021,0.00029692025,0.00007347484],"domain_scores_gemma":[0.996828,0.00143097,0.0004923076,0.00062211667,0.00053027505,0.00009628629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078177196,0.0003546635,0.00021932136,0.00042385588,0.0002664291,0.0005017194,0.00032972023,0.0002887105,0.0011316808],"category_scores_gemma":[0.002332054,0.0001960237,0.00022625114,0.0007623404,0.000282414,0.00037019278,0.00037029534,0.00049575727,0.00019993415],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021141018,0.0003178284,0.3668476,0.000194665,0.00029418865,0.0008395097,0.00030772746,0.11820384,0.4182016,0.003349657,0.0033697786,0.08595946],"study_design_scores_gemma":[0.00006479881,0.00042523566,0.63721305,0.000036583056,0.00023541077,0.00076127786,0.00011795975,0.14785312,0.20798668,0.0011709208,0.004063821,0.000071091396],"about_ca_topic_score_codex":0.0017046916,"about_ca_topic_score_gemma":0.0017368508,"teacher_disagreement_score":0.0017046916,"about_ca_system_score_codex":0.00038128626,"about_ca_system_score_gemma":0.00014153129,"threshold_uncertainty_score":0.004134476},"labels":[],"label_agreement":null},{"id":"W2949623359","doi":"10.3847/1538-4357/ab0205","title":"Influence of Stellar Metallicity on Occurrence Rates of Planets and Planetary Systems","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Planet; Metallicity; Physics; Astrophysics; Stars; Planetary system; RADIUS; Terrestrial planet; Astronomy; Star (game theory); Astrobiology","score_opus":0.011206928800093125,"score_gpt":0.22656069476958257,"score_spread":0.21535376596948944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949623359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99844366,0.00020646345,0.00016239074,0.00002888038,0.0000026748412,0.0000020187679,0.00028561085,0.000017683507,0.00085070764],"genre_scores_gemma":[0.99950206,0.000046586592,0.000040633473,0.0000062962595,0.0000033402432,7.111788e-7,0.00022156759,0.000008003724,0.00017077535],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996911,0.00007799899,0.000022429886,0.000110899105,0.00004445961,0.000053137355],"domain_scores_gemma":[0.9952101,0.002757518,0.0008113411,0.00045841452,0.000337455,0.00042521878],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000621275,0.00023737937,0.0003219791,0.00071709463,0.00021248177,0.000748484,0.00021768076,0.00031502548,0.00177774],"category_scores_gemma":[0.0041258098,0.0001557612,0.00027961985,0.00038864385,0.00038517785,0.0002981568,0.00031488374,0.00022915314,0.00051742507],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003161979,0.000023051618,0.9765406,0.00002133769,0.00010920215,0.00013571334,0.0000753769,0.0020216315,0.016428273,0.00012040141,0.00013173839,0.004076487],"study_design_scores_gemma":[0.0000045463844,0.00006924153,0.9926891,0.0000046552195,0.0000307861,0.00017992697,0.000055350814,0.0026647816,0.0038498014,0.00008601483,0.000359884,0.0000059287604],"about_ca_topic_score_codex":0.0016072186,"about_ca_topic_score_gemma":0.0014548488,"teacher_disagreement_score":0.00177774,"about_ca_system_score_codex":0.00021819524,"about_ca_system_score_gemma":0.00007636717,"threshold_uncertainty_score":0.005947113},"labels":[],"label_agreement":null},{"id":"W2949717157","doi":"10.3847/1538-4357/aaff5f","title":"Submillimeter Polarization Spectrum of the Carina Nebula","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Nebula; Vela; Radiative transfer; Molecular cloud; Planck; Telescope; Linear polarization; Astronomy; Optics; Stars; Pulsar; Laser","score_opus":0.005266924769628341,"score_gpt":0.20236897315315303,"score_spread":0.1971020483835247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949717157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99289906,0.00011428784,0.0006564704,0.000050415896,0.0000053492304,0.0000055819805,0.0010416557,0.00007637544,0.005150807],"genre_scores_gemma":[0.9980032,0.000036732232,0.0003279214,0.000025722367,0.0000059770978,0.0000044003177,0.00096343143,0.000010710394,0.00062203215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999938,0.0000046493287,0.0000010913094,0.000022991724,0.0000140552165,0.00001916615],"domain_scores_gemma":[0.99989533,0.000020209449,0.000018265448,0.000011379605,0.000034687986,0.000020123365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010608144,0.00018861069,0.00012837931,0.0006749462,0.00027808,0.00037950106,0.00018871916,0.00020406046,0.0020600155],"category_scores_gemma":[0.00014067837,0.000107662025,0.00010092685,0.00044024625,0.000117866584,0.00013333328,0.00022393481,0.00022487517,0.0003431336],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083498086,0.00014632304,0.46767846,0.000106433814,0.0001698778,0.00059825386,0.0010180747,0.0038225185,0.45737496,0.0009059125,0.0035715369,0.06377262],"study_design_scores_gemma":[0.000007338064,0.000032458087,0.98371744,0.0000072985335,0.000019516696,0.00008166479,0.0001059675,0.0019567593,0.011841122,0.00008933524,0.0021317455,0.000009387603],"about_ca_topic_score_codex":0.0049954774,"about_ca_topic_score_gemma":0.0069294875,"teacher_disagreement_score":0.0049954774,"about_ca_system_score_codex":0.0003230054,"about_ca_system_score_gemma":0.00009447199,"threshold_uncertainty_score":0.009932756},"labels":[],"label_agreement":null},{"id":"W2949725814","doi":"10.3847/1538-4357/aaa768","title":"Non-blackbody Disks Can Help Explain Inferred AGN Accretion Disk Sizes","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Physics; Black-body radiation; Accretion disc; Astrophysics; Accretion (finance); Astronomy; Radiation; Optics","score_opus":0.014158885229510528,"score_gpt":0.25190324050185936,"score_spread":0.23774435527234883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949725814","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93085694,0.0008737634,0.055404816,0.00085301895,0.00005506577,0.00003686432,0.0006141294,0.00032757252,0.010977995],"genre_scores_gemma":[0.9972697,0.00008733432,0.0019451942,0.00003065115,0.00001681107,0.000005156267,0.00007438856,0.000029278175,0.0005414565],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998826,0.00002250099,0.00000921375,0.000032172768,0.0000247408,0.000028764278],"domain_scores_gemma":[0.99895513,0.0004982695,0.00023298564,0.00013560557,0.00007892923,0.00009907708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039408598,0.00049038103,0.00041307742,0.00055188657,0.0003816403,0.0008656089,0.0010013102,0.00062869024,0.0027291416],"category_scores_gemma":[0.0029915387,0.00030966758,0.00047575452,0.00026821037,0.0005472761,0.0013084249,0.0007523628,0.00049440924,0.00039966186],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027095794,0.00019214171,0.3643857,0.0004323471,0.00020917639,0.0041125026,0.00063195324,0.3756421,0.09485612,0.11910642,0.005360219,0.034800295],"study_design_scores_gemma":[0.000044693938,0.000036949747,0.089621276,0.000035120036,0.000052915155,0.00081151654,0.00020526024,0.85501426,0.0068029435,0.04499103,0.0023465152,0.000037511334],"about_ca_topic_score_codex":0.0053527122,"about_ca_topic_score_gemma":0.0035590695,"teacher_disagreement_score":0.0053527122,"about_ca_system_score_codex":0.0008697688,"about_ca_system_score_gemma":0.00036372442,"threshold_uncertainty_score":0.010643125},"labels":[],"label_agreement":null},{"id":"W2949751374","doi":"10.3847/1538-4357/ab2333","title":"Evolutionary Models for Ultracool Dwarfs","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astrometry; Brown dwarf; Cover (algebra); Boundary (topology); Metallicity; Limit (mathematics); Exoplanet","score_opus":0.011792059659689718,"score_gpt":0.2233608782315305,"score_spread":0.2115688185718408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949751374","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5531573,0.0014077295,0.40644786,0.0013528154,0.00013978372,0.000106222345,0.0022375507,0.0012703695,0.033880305],"genre_scores_gemma":[0.9342993,0.0009878296,0.049507782,0.0002598324,0.00010490141,0.00021958679,0.0016931184,0.00047083545,0.012456841],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99975723,0.00007265394,0.000014204203,0.000075250595,0.000041681677,0.00003900715],"domain_scores_gemma":[0.9994048,0.00022543549,0.00010801349,0.000070437294,0.00009870483,0.00009261608],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005467612,0.00054610334,0.0007073919,0.0010198278,0.0009861079,0.0015296894,0.0019854666,0.0010767381,0.002788462],"category_scores_gemma":[0.0022840502,0.00039879754,0.00081315776,0.000715913,0.000732294,0.00120827,0.0012852442,0.000858703,0.00084289163],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000338776,0.000030231007,0.015221948,0.00004204259,0.000049778286,0.00018843061,0.00040116647,0.90775555,0.001781391,0.065654345,0.0012812072,0.0075599877],"study_design_scores_gemma":[0.000013055781,0.0000072309654,0.002197247,0.000009605288,0.000010769474,0.000064211774,0.00002854959,0.9739711,0.00012332501,0.020431142,0.003130859,0.000012933169],"about_ca_topic_score_codex":0.016172701,"about_ca_topic_score_gemma":0.0073202834,"teacher_disagreement_score":0.016172701,"about_ca_system_score_codex":0.0013359931,"about_ca_system_score_gemma":0.000546139,"threshold_uncertainty_score":0.032157123},"labels":[],"label_agreement":null},{"id":"W2949779906","doi":"10.1086/496911","title":"Intrinsic Absorption in the Spectrum of NGC 7469: Simultaneous<i>Chandra</i>,<i>FUSE</i>, and STIS Observations","year":2005,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Space Telescope Imaging Spectrograph; Astrophysics; Galaxy; Ultraviolet; Absorption (acoustics); Spectral line; Absorption spectroscopy; Photoionization; Ionization; Line (geometry); Emission spectrum; Astronomy; Hubble space telescope; Optics; Ion","score_opus":0.013615027038456564,"score_gpt":0.2252191380900612,"score_spread":0.21160411105160462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949779906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99762136,0.000083196406,0.00022006193,0.000014698811,0.0000070232627,0.0000026681435,0.0006093066,0.00010861841,0.0013330005],"genre_scores_gemma":[0.99874264,0.000048837188,0.00050821254,0.000009669676,0.000010157612,0.0000026996224,0.00052298437,0.000009810886,0.00014513168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999057,0.00000471597,0.0000040694385,0.000025231615,0.000027794747,0.00003254109],"domain_scores_gemma":[0.9998543,0.000012430238,0.000057001707,0.000012815719,0.000018548679,0.000044806013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000071139446,0.00029830495,0.00021362647,0.0010922633,0.00047871275,0.00036616466,0.000254583,0.00027727627,0.0011913367],"category_scores_gemma":[0.00018880448,0.00013443937,0.0002105385,0.0006463077,0.00023395952,0.00023762576,0.00025487394,0.00023935549,0.00022681337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005381318,0.0002228892,0.720672,0.00012791311,0.00022616376,0.0016154343,0.0005832776,0.006414766,0.23757873,0.0010988797,0.003056634,0.027865179],"study_design_scores_gemma":[0.000009281835,0.000067987035,0.9917116,0.000007998955,0.000040503364,0.00051077077,0.000059953614,0.001755095,0.0043104407,0.00009044027,0.001419429,0.000016404498],"about_ca_topic_score_codex":0.012395045,"about_ca_topic_score_gemma":0.020673519,"teacher_disagreement_score":0.012395045,"about_ca_system_score_codex":0.00041027437,"about_ca_system_score_gemma":0.00016572498,"threshold_uncertainty_score":0.024645805},"labels":[],"label_agreement":null},{"id":"W2949783635","doi":"10.1088/0004-637x/712/1/367","title":"ESTIMATING SMALL ANGULAR SCALE COSMIC MICROWAVE BACKGROUND ANISOTROPY WITH HIGH-RESOLUTION<i>N</i>-BODY SIMULATIONS: WEAK LENSING","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Saint Mary's University","funders":"","keywords":"Cosmic microwave background; Weak gravitational lensing; Gravitational lens; Cosmic variance; Strong gravitational lensing; Gravitational lensing formalism; Spectral density; Cosmic background radiation; COSMIC cancer database","score_opus":0.00872639466389157,"score_gpt":0.2376156684915128,"score_spread":0.22888927382762123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949783635","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94896924,0.00009466045,0.043392397,0.00021641269,0.000034626395,0.00003843304,0.00033343254,0.00077446434,0.0061463914],"genre_scores_gemma":[0.96505076,0.000045868954,0.033790875,0.00004987421,0.000015306101,0.00004180321,0.00034902737,0.00021629233,0.0004401608],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982196,0.00005783788,0.000009843505,0.000023213266,0.000049596732,0.000037565325],"domain_scores_gemma":[0.997928,0.0012395263,0.00025445194,0.00019253108,0.00022993954,0.00015547633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008661064,0.00051895576,0.00044778726,0.00046254165,0.0004185504,0.0005779551,0.0009860148,0.0005021428,0.0010316923],"category_scores_gemma":[0.0040631583,0.00027747857,0.0004638461,0.0005178603,0.00053649925,0.00048689364,0.0005227946,0.0007850208,0.00014229094],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019482334,0.00011724742,0.024801925,0.00004897426,0.00008609411,0.00012097618,0.000106496,0.95892274,0.00476462,0.0034682495,0.00065341004,0.0067144833],"study_design_scores_gemma":[0.000011302226,0.0000086894925,0.0012351475,0.0000018833665,0.0000032059793,0.0000041741137,0.000007632889,0.99760604,0.00080959924,0.00021308353,0.00009635997,0.0000029042494],"about_ca_topic_score_codex":0.014830436,"about_ca_topic_score_gemma":0.010131283,"teacher_disagreement_score":0.014830436,"about_ca_system_score_codex":0.000595264,"about_ca_system_score_gemma":0.0007117114,"threshold_uncertainty_score":0.029488206},"labels":[],"label_agreement":null},{"id":"W2949827927","doi":"10.3847/1538-4357/aaf9b3","title":"Blue Straggler Stars beyond the Milky Way. IV. Radial Distributions and Dynamical Implications","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Blue straggler; Milky Way; Stars; Astronomy; Astrophysics; Radial velocity; Star cluster","score_opus":0.0072210102879378645,"score_gpt":0.2208195079413418,"score_spread":0.21359849765340394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2949827927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99870443,0.00019342928,0.00021175177,0.000038284517,0.0000015057392,0.0000011615218,0.00006555155,0.000007987123,0.00077591103],"genre_scores_gemma":[0.9997032,0.000031704258,0.000047678313,0.0000028742543,0.0000018651831,3.0281967e-7,0.00003680993,0.0000016945959,0.00017378456],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993277,0.000009233644,0.0000036383726,0.000024674368,0.000009343664,0.000020340025],"domain_scores_gemma":[0.9992291,0.00012847947,0.00026968686,0.00005854466,0.00012921145,0.00018497552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003196613,0.00017225838,0.0001833068,0.001076153,0.00036833461,0.0006158204,0.0003188426,0.00017397242,0.0012803338],"category_scores_gemma":[0.0011015733,0.00008619449,0.00015885796,0.00053684483,0.00056892826,0.000554435,0.00051983056,0.00019634396,0.00020111],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008686484,0.0000131528195,0.9790754,0.000016158137,0.000024175732,0.00021201011,0.00032387208,0.002135051,0.007650234,0.0025098324,0.00011945831,0.00783379],"study_design_scores_gemma":[0.000002756443,0.00002951933,0.99397534,0.000007064237,0.000008611943,0.00014823329,0.00033738173,0.002748555,0.00069698883,0.0016164227,0.00042409648,0.0000051021243],"about_ca_topic_score_codex":0.0069305734,"about_ca_topic_score_gemma":0.0067962795,"teacher_disagreement_score":0.0069305734,"about_ca_system_score_codex":0.00053533696,"about_ca_system_score_gemma":0.00015931942,"threshold_uncertainty_score":0.013780415},"labels":[],"label_agreement":null},{"id":"W2950007064","doi":"10.1088/0004-637x/742/1/4","title":"ON THE EXTENDED EMISSION AROUND THE ANOMALOUS X-RAY PULSAR 1E 1547.0–5408","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Flux (metallurgy); Pulsar wind nebula; Halo; Supernova remnant; Supernova; Nebula; Emission spectrum","score_opus":0.023792306095283874,"score_gpt":0.23192131576006159,"score_spread":0.2081290096647777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950007064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99916196,0.00009956433,0.00016239307,0.000008915995,0.0000016022859,0.0000019928093,0.00008851711,0.0000064711207,0.00046857825],"genre_scores_gemma":[0.9989963,0.00010148461,0.00039896442,0.000006380841,0.000014486229,0.000004210092,0.0003679697,0.000005305302,0.00010484056],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991524,0.0000137984125,0.000004861835,0.000024518791,0.00002117766,0.000020383146],"domain_scores_gemma":[0.9995654,0.00012130769,0.00017292348,0.00003767105,0.000047994894,0.000054680422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001951206,0.00024338713,0.0002318307,0.0012376833,0.00022127118,0.00030320196,0.00019777929,0.00016543557,0.0006938184],"category_scores_gemma":[0.00050902134,0.00010861628,0.0002165579,0.00064351474,0.00030201682,0.00022327753,0.0004828502,0.00013801685,0.00017831092],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004725769,0.00007271848,0.87227005,0.0000890793,0.00016501831,0.0017824053,0.00037720386,0.0013367446,0.09977073,0.00036397876,0.00031659822,0.022982853],"study_design_scores_gemma":[0.00000487232,0.000045611232,0.99690634,0.000007969056,0.000030457493,0.0005748272,0.000040120696,0.0007167245,0.0012153388,0.00008019278,0.00037348433,0.0000040096425],"about_ca_topic_score_codex":0.00069235364,"about_ca_topic_score_gemma":0.0019589085,"teacher_disagreement_score":0.0012376833,"about_ca_system_score_codex":0.0001645136,"about_ca_system_score_gemma":0.000055830114,"threshold_uncertainty_score":0.0023210645},"labels":[],"label_agreement":null},{"id":"W2950014879","doi":"10.1088/0004-637x/752/2/88","title":"SEMI-BLIND EIGEN ANALYSES OF RECOMBINATION HISTORIES USING COSMIC MICROWAVE BACKGROUND DATA","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cosmic microwave background; Redshift; Cosmology; Recombination; Cosmic background radiation; COSMIC cancer database; Visibility","score_opus":0.10355299446289132,"score_gpt":0.36035779032792914,"score_spread":0.2568047958650378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950014879","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6963765,0.00015015143,0.2988832,0.00009641912,0.0000142924955,0.000032839762,0.0015981913,0.0009139507,0.0019345182],"genre_scores_gemma":[0.9227891,0.00006922254,0.07466615,0.000027587233,0.00001625537,0.000023371576,0.0015591723,0.00017747318,0.0006716041],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99952364,0.00017307067,0.000032102293,0.000110968955,0.00008367522,0.00007668883],"domain_scores_gemma":[0.9979201,0.0008246158,0.00033073412,0.0005918068,0.00017367968,0.00015915417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014562233,0.00050591014,0.0002342745,0.001972561,0.000368154,0.00090253475,0.00052882556,0.00028339334,0.0012924013],"category_scores_gemma":[0.004173844,0.00020255292,0.0006181676,0.00072553556,0.00036235544,0.00075186364,0.0009807528,0.00045095134,0.0005189914],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016688277,0.0002737428,0.29447827,0.00028156472,0.0005821141,0.00039969943,0.0012739593,0.197215,0.1230236,0.056503322,0.003260241,0.3210397],"study_design_scores_gemma":[0.000044587785,0.00009238275,0.13139053,0.000061140345,0.0000832583,0.00018079662,0.00029410486,0.7937385,0.035713483,0.03505384,0.0032443549,0.00010305284],"about_ca_topic_score_codex":0.0022491834,"about_ca_topic_score_gemma":0.0030208775,"teacher_disagreement_score":0.0022491834,"about_ca_system_score_codex":0.00029640607,"about_ca_system_score_gemma":0.00036235387,"threshold_uncertainty_score":0.0077012777},"labels":[],"label_agreement":null},{"id":"W2950067845","doi":"10.3847/1538-4357/ab2985","title":"KSP-OT-201611a: A Distant Population II Dwarf Nova Candidate Discovered by the KMTNet Supernova Program","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Gravitational microlensing; Dwarf nova; Accretion (finance); Population; Supernova; White dwarf; Dwarf galaxy; Cataclysmic variable star","score_opus":0.009453229085712106,"score_gpt":0.2434396202326572,"score_spread":0.23398639114694508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950067845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978811,0.00015423191,0.0002200097,0.000038943537,0.000025371824,0.000014755074,0.00031983817,0.000011096229,0.0013347394],"genre_scores_gemma":[0.9980192,0.000075505035,0.00029369438,0.000033325203,0.00001793241,0.0000035661546,0.0007672216,0.000005850381,0.00078368513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998827,0.000005424146,0.000011003822,0.000040175677,0.000027432076,0.000033328222],"domain_scores_gemma":[0.9996008,0.000012174017,0.00006534101,0.000021477526,0.000025928,0.00027432098],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014413543,0.00036292415,0.00032318773,0.0008900503,0.0008608736,0.0005753488,0.00024695086,0.00030272768,0.0014622333],"category_scores_gemma":[0.0002079289,0.00014615439,0.00034196596,0.00042625458,0.00027139825,0.00026481817,0.00071794324,0.00039909818,0.0003540873],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040715016,0.00019517793,0.9128095,0.00005957259,0.000078311095,0.030105235,0.000247362,0.0002541937,0.043153327,0.0005024614,0.000950562,0.011237173],"study_design_scores_gemma":[0.000019509145,0.00029814139,0.9396802,0.00001765125,0.000039572475,0.04836004,0.00035177512,0.00078850274,0.0051094415,0.00027692685,0.0050397418,0.000018516514],"about_ca_topic_score_codex":0.002244956,"about_ca_topic_score_gemma":0.0041535567,"teacher_disagreement_score":0.002244956,"about_ca_system_score_codex":0.0002845163,"about_ca_system_score_gemma":0.00020322573,"threshold_uncertainty_score":0.004891634},"labels":[],"label_agreement":null},{"id":"W2950163788","doi":"10.3847/1538-4357/ab13a2","title":"JCMT BISTRO Survey: Magnetic Fields within the Hub-filament Structure in IC 5146","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Dalhousie University; Western University; University of Manitoba; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Ministry of Science and Technology, Taiwan","keywords":"James Clerk Maxwell Telescope; Magnetic field; Polarization (electrochemistry); Polarimeter; Bolometer; Polarimetry; Dynamo; Protostar","score_opus":0.007882057145779515,"score_gpt":0.22441936192993325,"score_spread":0.21653730478415373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950163788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964664,0.0001262285,0.00018597505,0.000031698975,0.000004188974,0.000010576967,0.0012654881,0.000060519826,0.0018489772],"genre_scores_gemma":[0.99803895,0.00005942161,0.00024278526,0.000020650252,0.00001737248,0.0000054888046,0.0013946514,0.000009301834,0.0002114747],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980897,0.00001656246,0.000010694855,0.000049788112,0.00005270547,0.000061334285],"domain_scores_gemma":[0.9993788,0.000034827674,0.00024086575,0.00008674326,0.00007347623,0.00018521189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018094527,0.00025437918,0.0002770054,0.0015875953,0.00039396939,0.0005316031,0.0003079403,0.00031688888,0.0011722518],"category_scores_gemma":[0.00053439836,0.00012785192,0.00021298298,0.00089199876,0.00023501882,0.00023771595,0.0004811539,0.00019288552,0.00031566044],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026951407,0.00008668859,0.9346575,0.00004595473,0.00010079759,0.00067967817,0.0003426917,0.0013621463,0.047311056,0.00028744753,0.0017538018,0.013102738],"study_design_scores_gemma":[0.000005067689,0.0000153657,0.9978198,0.000003805585,0.00000992052,0.0001355918,0.000035959172,0.00059440616,0.0007584245,0.000012531113,0.0006059084,0.000003274443],"about_ca_topic_score_codex":0.015972756,"about_ca_topic_score_gemma":0.016773878,"teacher_disagreement_score":0.015972756,"about_ca_system_score_codex":0.0004290506,"about_ca_system_score_gemma":0.00022801265,"threshold_uncertainty_score":0.03175956},"labels":[],"label_agreement":null},{"id":"W2950205458","doi":"10.1086/521049","title":"Eccentric Double White Dwarfs as <i>LISA</i> Sources in Globular Clusters","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Eccentricity (behavior); Population; Neutron star; Stars; Orbital eccentricity; Astronomy","score_opus":0.008424745194458173,"score_gpt":0.2270102215837505,"score_spread":0.21858547638929232,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950205458","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977119,0.00021897044,0.0007527457,0.00003652359,0.0000029354733,0.0000029256887,0.000028206558,0.000012528503,0.0012332315],"genre_scores_gemma":[0.99952364,0.000056014254,0.00022252148,0.0000063664675,0.000006030583,0.0000012212407,0.00004406125,0.0000023830257,0.00013773247],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999018,0.0000131509,0.0000043436517,0.000032694817,0.00001968739,0.00002847334],"domain_scores_gemma":[0.99946254,0.00010831176,0.00022512923,0.000040854742,0.00004477838,0.00011827181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027232358,0.0002686526,0.00021955738,0.0009312441,0.0008333145,0.0008826055,0.00031999368,0.0003425711,0.00053275714],"category_scores_gemma":[0.0009626829,0.00014781719,0.0001015169,0.0010841824,0.0006600073,0.00040534322,0.0007803689,0.00012891821,0.0001294058],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022249568,0.000046103425,0.9436096,0.000042461044,0.000057989782,0.0013896925,0.00070542307,0.011547796,0.011380165,0.017033884,0.00090211356,0.013062314],"study_design_scores_gemma":[0.000026695734,0.00011455263,0.93378687,0.000027491791,0.00011831906,0.0025615788,0.0009885927,0.038521115,0.0040564537,0.016134934,0.003625812,0.00003758926],"about_ca_topic_score_codex":0.0036912847,"about_ca_topic_score_gemma":0.0040457556,"teacher_disagreement_score":0.0036912847,"about_ca_system_score_codex":0.0004475899,"about_ca_system_score_gemma":0.00022395788,"threshold_uncertainty_score":0.0073395967},"labels":[],"label_agreement":null},{"id":"W2950281463","doi":"10.3847/1538-4357/ab13a4","title":"Discovery of a Double Blue Straggler Sequence in M15: New Insight into the Core-collapse Process","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Blue straggler; Sequence (biology); Cluster (spacecraft); Diagram; Population; Event (particle physics); Star cluster; Set (abstract data type)","score_opus":0.01852246713566086,"score_gpt":0.26936263758160967,"score_spread":0.2508401704459488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950281463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986099,0.00024333107,0.00076221535,0.000011165647,0.0000032827913,0.0000045014876,0.000034796067,0.000017793358,0.000312938],"genre_scores_gemma":[0.99855,0.000060588678,0.0010926289,0.000015059063,0.00000534382,0.0000021957947,0.00009936187,0.000004204697,0.00017056744],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995446,0.0000030899816,0.0000027973917,0.000015210293,0.0000119742035,0.000012582688],"domain_scores_gemma":[0.99982136,0.000015679709,0.000049897295,0.000021317039,0.000019915462,0.0000717806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011480346,0.00018188193,0.00018415698,0.0008912699,0.00022093664,0.00026757846,0.00029866237,0.0003060843,0.00080957456],"category_scores_gemma":[0.00018742212,0.000106100146,0.00017570771,0.00027909543,0.0002665132,0.00021480561,0.000423908,0.000186774,0.00024754164],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035078672,0.000061519415,0.3312784,0.00011355365,0.000049620976,0.0026135705,0.0006975123,0.0005735514,0.64549446,0.0007450735,0.00016514116,0.017856784],"study_design_scores_gemma":[0.0000057957527,0.00024707706,0.95375335,0.000017264794,0.00002642573,0.0035923866,0.00022548709,0.0027042006,0.03621674,0.00052936154,0.0026628333,0.000019001674],"about_ca_topic_score_codex":0.00084384193,"about_ca_topic_score_gemma":0.0016148677,"teacher_disagreement_score":0.0008912699,"about_ca_system_score_codex":0.00018841584,"about_ca_system_score_gemma":0.00009591363,"threshold_uncertainty_score":0.0027083158},"labels":[],"label_agreement":null},{"id":"W2950295486","doi":"10.3847/1538-4357/ab11d2","title":"Initial Mass Function Variation in Two Elliptical Galaxies Using Near-infrared Tracers","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Initial mass function; Stellar population; Milky Way; Galaxy; Population; Spectral line; Absorption (acoustics)","score_opus":0.01016095862115107,"score_gpt":0.23690537966716918,"score_spread":0.2267444210460181,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950295486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99950516,0.000022569593,0.00030892948,0.0000027626813,3.2436952e-7,9.2926905e-7,0.000021248465,0.000010626476,0.00012740571],"genre_scores_gemma":[0.99968386,0.000006746877,0.00022588046,0.0000017077625,4.2305578e-7,5.6937273e-7,0.000042826312,0.0000011916784,0.00003675092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993956,0.000009951024,0.000003090867,0.00002050028,0.000013118926,0.000013732975],"domain_scores_gemma":[0.9995932,0.00009103168,0.00015236567,0.000041306022,0.000056538924,0.00006561746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035699838,0.00016879433,0.00015431717,0.0011523531,0.00015491722,0.0003883024,0.00021205128,0.00022899699,0.0002695462],"category_scores_gemma":[0.00063348754,0.00009846886,0.00014956776,0.00035840878,0.00020566199,0.00024012306,0.00028415982,0.00013237796,0.00009938389],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020648888,0.00005112606,0.9310594,0.000012509542,0.000043774875,0.00014603806,0.0003257495,0.0018535174,0.058865186,0.00044923023,0.000044348024,0.006942612],"study_design_scores_gemma":[0.0000032103221,0.00004149546,0.9858731,0.0000033789356,0.000013150851,0.000081856386,0.00009908403,0.009224001,0.004367662,0.00012931511,0.00015903194,0.0000047024437],"about_ca_topic_score_codex":0.0025875312,"about_ca_topic_score_gemma":0.0027016902,"teacher_disagreement_score":0.0025875312,"about_ca_system_score_codex":0.00034248194,"about_ca_system_score_gemma":0.00005516519,"threshold_uncertainty_score":0.0051450133},"labels":[],"label_agreement":null},{"id":"W2950338157","doi":"10.3847/1538-4357/ab253d","title":"The Ultracool SpeXtroscopic Survey. I. Volume-limited Spectroscopic Sample and Luminosity Function of M7−L5 Ultracool Dwarfs","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Sample (material); Luminosity function; Volume (thermodynamics); Function (biology); Brown dwarf; Physics; Luminosity; Astrophysics; Stars; Biology","score_opus":0.009515653806879174,"score_gpt":0.21830445471799392,"score_spread":0.20878880091111474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950338157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99796766,0.00011069683,0.000099500816,0.000011453888,9.958682e-7,0.0000033777774,0.0011859207,0.000014137136,0.0006062338],"genre_scores_gemma":[0.99499077,0.0000680457,0.0002702236,0.000019288329,0.0000063983243,0.0000070837923,0.004294766,0.000008016179,0.00033533247],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996898,0.000036622805,0.000027376635,0.000075646,0.00009311096,0.000077459685],"domain_scores_gemma":[0.9988304,0.00010523482,0.0003818544,0.0001468296,0.00019938205,0.00033633068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040666672,0.0001835359,0.00026254478,0.0021812401,0.00034089622,0.0004764307,0.0004245781,0.00013608641,0.0010135522],"category_scores_gemma":[0.00097196916,0.00009323551,0.000188068,0.0011150414,0.00026267848,0.00024651614,0.0008057549,0.00009285487,0.0005964382],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001054334,0.000020534835,0.98578227,0.00002728931,0.00003791066,0.000114617156,0.0004243989,0.00012687579,0.0033108518,0.0002281074,0.0007708771,0.00905083],"study_design_scores_gemma":[0.000004759754,0.00004389621,0.996612,0.000011109968,0.000012432919,0.00013257,0.0002528545,0.00040935812,0.0006957777,0.00003720978,0.0017850817,0.0000029862347],"about_ca_topic_score_codex":0.010699868,"about_ca_topic_score_gemma":0.016792709,"teacher_disagreement_score":0.010699868,"about_ca_system_score_codex":0.00033837016,"about_ca_system_score_gemma":0.00027646322,"threshold_uncertainty_score":0.021275163},"labels":[],"label_agreement":null},{"id":"W2950354986","doi":"10.3847/1538-4357/ab153a","title":"On the Measurement of Fundamental Parameters of White Dwarfs in the Gaia Era","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"White dwarf; Parallax; Sky; Brown dwarf; Stars; Diagram; Stellar evolution; Massive compact halo object","score_opus":0.019472675904058302,"score_gpt":0.22028324575922495,"score_spread":0.20081056985516665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950354986","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.009383243,0.9770498,0.0068371682,0.0013285796,0.00080241746,0.000022549746,0.00046481256,0.00015838162,0.003952874],"genre_scores_gemma":[0.09273306,0.8814175,0.016924016,0.002273948,0.003238565,0.00007226188,0.0011552599,0.00023560657,0.0019497252],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9983677,0.00024894183,0.00015080378,0.00049557263,0.0006541663,0.000082715254],"domain_scores_gemma":[0.99462056,0.0019995458,0.0007030213,0.0004196329,0.002122244,0.00013498524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004670794,0.0010541566,0.0010827262,0.0058780224,0.00045528487,0.0020418717,0.001229557,0.0005983083,0.00042090492],"category_scores_gemma":[0.0075066187,0.00052052963,0.0005149029,0.0036559554,0.0016141344,0.0021431758,0.0009603322,0.0014130487,0.0005066118],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022523034,0.000056583358,0.03759023,0.0077704173,0.0005167738,0.00019508539,0.00039292782,0.0022674385,0.01661852,0.017399447,0.02221372,0.89475363],"study_design_scores_gemma":[0.000016798424,0.0002453447,0.113816954,0.0036592605,0.00047721883,0.0009228012,0.00026861587,0.0012588872,0.011630641,0.010208678,0.85735846,0.00013629353],"about_ca_topic_score_codex":0.007423132,"about_ca_topic_score_gemma":0.0058918195,"teacher_disagreement_score":0.007423132,"about_ca_system_score_codex":0.0025738531,"about_ca_system_score_gemma":0.001176706,"threshold_uncertainty_score":0.024701834},"labels":[],"label_agreement":null},{"id":"W2950360321","doi":"10.3847/1538-4357/aadcab","title":"A Multiwavelength View of the Neutron Star Binary 1FGL J1417.7–4402: A Progenitor to Canonical Millisecond Pulsars","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Millisecond pulsar; Neutron star; Pulsar; Binary pulsar; Accretion (finance); X-ray pulsar; Pulsar planet; Luminosity; Binary number","score_opus":0.01384750806893683,"score_gpt":0.24925349378665757,"score_spread":0.23540598571772073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950360321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98155403,0.0006553144,0.00084993645,0.00020304856,0.000020573976,0.000009053858,0.00030436815,0.00009085511,0.01631272],"genre_scores_gemma":[0.9956802,0.00018668911,0.0018472144,0.00007398941,0.000034687135,0.0000062878457,0.000254161,0.00003147481,0.0018853827],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999752,0.0000022735169,8.749804e-7,0.000005639112,0.000006889333,0.000009158866],"domain_scores_gemma":[0.9999138,0.00001251004,0.000020599307,0.0000060050165,0.00001216404,0.000034883724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000069608875,0.00012907934,0.00012845328,0.0010471122,0.00037335185,0.00036543913,0.00026922417,0.00036360484,0.0025684335],"category_scores_gemma":[0.00008476406,0.00014925504,0.00015314945,0.0002519039,0.00014226924,0.00021287316,0.00044165817,0.00035097805,0.00057103374],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064907374,0.00028692893,0.19476333,0.000199049,0.00010999136,0.014160772,0.0009678127,0.0025137975,0.7333402,0.0044199903,0.0038578634,0.04473124],"study_design_scores_gemma":[0.000028422259,0.00015618831,0.9699879,0.000050682942,0.00003895465,0.0060631204,0.0005010738,0.0047410727,0.0079107,0.0009305149,0.009575211,0.000016115448],"about_ca_topic_score_codex":0.0020389587,"about_ca_topic_score_gemma":0.003943217,"teacher_disagreement_score":0.0025684335,"about_ca_system_score_codex":0.00031605762,"about_ca_system_score_gemma":0.00007778079,"threshold_uncertainty_score":0.008592248},"labels":[],"label_agreement":null},{"id":"W2950387337","doi":"10.3847/1538-4357/ab1b11","title":"Discovery of a White Dwarf Companion to HD 159062","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Observatory; Photometry (optics); Radial velocity; Telescope; Orbital period","score_opus":0.008896659128359444,"score_gpt":0.22144456879443292,"score_spread":0.21254790966607348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950387337","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99787295,0.00020424917,0.00041844792,0.000037916285,0.00003686229,0.000007918784,0.00025782213,0.000020844642,0.0011429675],"genre_scores_gemma":[0.9968983,0.00006975884,0.0010533354,0.00006648656,0.000043185224,0.0000051471256,0.0011996314,0.0000067708884,0.0006574519],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997836,0.000012217559,0.000022220916,0.00008063989,0.00007305174,0.000028327004],"domain_scores_gemma":[0.99939716,0.000080681784,0.00014599695,0.00007042856,0.00009108937,0.0002146919],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043733275,0.00022379225,0.0003293046,0.0010309671,0.0008660937,0.00055300654,0.00032766958,0.0007798594,0.0010149818],"category_scores_gemma":[0.00077268697,0.00014656819,0.00024141939,0.0005113834,0.00025477508,0.00031653317,0.00069965614,0.00043894092,0.0006538134],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004810212,0.0004317055,0.59292114,0.00015509373,0.00014209512,0.014669439,0.0012105715,0.0003695617,0.36344483,0.0011814717,0.0017369691,0.023256063],"study_design_scores_gemma":[0.000032404296,0.0010066334,0.9106205,0.000033812183,0.00006223497,0.029586509,0.00045603432,0.0016077375,0.03360882,0.00053806615,0.022414295,0.000032933967],"about_ca_topic_score_codex":0.0007401698,"about_ca_topic_score_gemma":0.0008786136,"teacher_disagreement_score":0.0010309671,"about_ca_system_score_codex":0.00024601695,"about_ca_system_score_gemma":0.00019556632,"threshold_uncertainty_score":0.0033954382},"labels":[],"label_agreement":null},{"id":"W2950407002","doi":"10.1088/0004-637x/738/1/112","title":"WARM H<sub>2</sub>O AND OH DISK EMISSION IN V1331 Cyg","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Spectral line; HITRAN; Emission spectrum; Line (geometry); Irradiation; Range (aeronautics); Thermal; Spectral resolution","score_opus":0.012851044831623146,"score_gpt":0.21935932923722476,"score_spread":0.20650828440560162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950407002","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990569,0.00006367201,0.00008798761,0.00004145418,0.0000016984529,0.0000028006116,0.00015309865,0.000029891318,0.0005626185],"genre_scores_gemma":[0.9990103,0.00005589245,0.00025420586,0.00004333871,0.00001086196,0.0000050379876,0.00044040388,0.00001583639,0.0001640233],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995065,0.0000026132163,0.0000011615225,0.000014746401,0.000008727542,0.000022069598],"domain_scores_gemma":[0.9998841,0.000013621607,0.000045178895,0.0000063646467,0.0000070292645,0.00004365204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008979683,0.00031857882,0.00024959136,0.00043951138,0.00036172036,0.0004702949,0.00025327055,0.00030765712,0.0010444546],"category_scores_gemma":[0.00015858238,0.00012108496,0.00015343506,0.00041813648,0.00025561327,0.00022762513,0.00043024446,0.00035652067,0.00024637964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010935909,0.00021022762,0.49318862,0.0002480195,0.0001238805,0.005871842,0.0019465409,0.007268537,0.45457742,0.0017139503,0.0032404903,0.030516867],"study_design_scores_gemma":[0.000015812644,0.000050927825,0.99278706,0.000009454813,0.000020033158,0.00031679566,0.00015944138,0.0023625751,0.0030501464,0.0002155477,0.0010007294,0.000011529117],"about_ca_topic_score_codex":0.0056173033,"about_ca_topic_score_gemma":0.008834836,"teacher_disagreement_score":0.0056173033,"about_ca_system_score_codex":0.0005885061,"about_ca_system_score_gemma":0.00015137167,"threshold_uncertainty_score":0.011169195},"labels":[],"label_agreement":null},{"id":"W2950443932","doi":"10.1086/339419","title":"[ITAL]Chandra[/ITAL] Imaging of the Gamma-Ray Source G[CLC]e[/CLC]V J1809−2327","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Pulsar; Astrophysics; Point source; Pulsar wind nebula; X-ray; Nebula; Astronomy; Stars; Optics","score_opus":0.006902673164496944,"score_gpt":0.19012380139919757,"score_spread":0.18322112823470063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950443932","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.69148326,0.005258771,0.0055343136,0.0025816557,0.0031537416,0.00020062248,0.044417053,0.0069156955,0.24045494],"genre_scores_gemma":[0.8636033,0.003450228,0.027288344,0.002028502,0.0012434064,0.000081703736,0.047229532,0.0015526745,0.053522356],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9999442,0.0000026719517,0.0000028229833,0.000012185261,0.00002061302,0.000017441469],"domain_scores_gemma":[0.99987185,0.0000085499705,0.00003242244,0.00002236108,0.000031507876,0.000033345856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006032044,0.000245059,0.00018789522,0.0016615267,0.00032777144,0.00046970058,0.0005162066,0.00023038522,0.033140387],"category_scores_gemma":[0.00024380613,0.0001689328,0.00023981188,0.0009331057,0.00017691292,0.00025790237,0.00041682317,0.0003292632,0.0050214333],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012853849,0.00019311062,0.0596722,0.0010177175,0.00022459001,0.0040484304,0.00020626672,0.0021478909,0.27017424,0.005977911,0.46899873,0.18605357],"study_design_scores_gemma":[0.0001543074,0.0001906409,0.43041462,0.00032009344,0.0001384764,0.0063430355,0.00022190872,0.0018690964,0.035266966,0.0016939404,0.52330154,0.000085321626],"about_ca_topic_score_codex":0.0046071336,"about_ca_topic_score_gemma":0.012813387,"teacher_disagreement_score":0.033140387,"about_ca_system_score_codex":0.00015688642,"about_ca_system_score_gemma":0.00020093634,"threshold_uncertainty_score":0.11086565},"labels":[],"label_agreement":null},{"id":"W2950509913","doi":"10.1088/0004-637x/753/1/33","title":"A POPULATION OF DUST-RICH QUASARS AT<i>z</i>∼ 1.5","year":2012,"lang":"fa","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Centre National de la Recherche Scientifique; Università degli Studi di Padova; Jet Propulsion Laboratory; Centre National d’Etudes Spatiales; Cardiff University; Imperial College London; University of Lethbridge; California Institute of Technology; National Aeronautics and Space Administration; UK Space Agency; University of Sussex; Smithsonian Institution","keywords":"Quasar; Astrophysics; Physics; Redshift; Galaxy; Infrared; Population; Astronomy; Luminous infrared galaxy","score_opus":0.010873175314881058,"score_gpt":0.2261985293648167,"score_spread":0.21532535404993564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950509913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985511,0.00008905806,0.00015457704,0.000028586815,0.0000028628706,0.000011791455,0.00032968918,0.000022824219,0.0008095652],"genre_scores_gemma":[0.9987368,0.00004329913,0.0001434474,0.00006195551,0.000013097725,0.000004932855,0.00057136704,0.000003236502,0.0004218575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998006,0.000012890917,0.000013832151,0.000071355746,0.000037953574,0.00006340147],"domain_scores_gemma":[0.99951637,0.000035893092,0.00018708107,0.000047836354,0.00005050522,0.00016226842],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003468374,0.00023459972,0.00023593867,0.0010254038,0.0005281491,0.0006775919,0.0003602011,0.00021390365,0.0020918187],"category_scores_gemma":[0.0004734114,0.0001296485,0.0001274037,0.00048861036,0.00033495395,0.000547431,0.00041515764,0.0002565068,0.0005805693],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000076316144,0.00009117659,0.9845238,0.0000096322465,0.00001788166,0.00029376193,0.0004581395,0.000043207452,0.008647959,0.00015430714,0.0003412742,0.0053425673],"study_design_scores_gemma":[0.000005526859,0.00007549146,0.9980482,0.0000014617049,0.000005497798,0.0006780108,0.00015215657,0.00007476246,0.00032950586,0.000060301772,0.0005654847,0.0000036027322],"about_ca_topic_score_codex":0.0027944832,"about_ca_topic_score_gemma":0.0040030982,"teacher_disagreement_score":0.0027944832,"about_ca_system_score_codex":0.00019555868,"about_ca_system_score_gemma":0.0000935696,"threshold_uncertainty_score":0.0069978237},"labels":[],"label_agreement":null},{"id":"W2950532479","doi":"10.3847/1538-4357/ab14f4","title":"A Search for Pulsed Very High-energy Gamma-Rays from 13 Young Pulsars in Archival VERITAS Data","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Pulsar; Flux (metallurgy); Crab Pulsar; Data set; Neutron star; Millisecond pulsar; High energy","score_opus":0.01957716110318723,"score_gpt":0.30307594409845917,"score_spread":0.2834987829952719,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950532479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968104,0.00008001578,0.00059957954,0.000015056301,0.0000028159027,0.000013562455,0.0018579476,0.000024430865,0.00059621845],"genre_scores_gemma":[0.98477256,0.0000940956,0.002825238,0.000025504552,0.000013997765,0.000039232138,0.011389669,0.00002056469,0.0008191744],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991166,0.000087501576,0.00009732281,0.00019376284,0.0003680923,0.00013669123],"domain_scores_gemma":[0.99628013,0.0011965471,0.0009992435,0.00066089444,0.0005499691,0.00031308303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014855037,0.00023066656,0.00041204935,0.0032825102,0.00070388656,0.0012077758,0.00048552777,0.0003903139,0.001792074],"category_scores_gemma":[0.002347307,0.00022968621,0.00029343466,0.002034847,0.00043484912,0.00036516698,0.0012982121,0.0003700407,0.00038882098],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004966054,0.00008757418,0.93573636,0.00007882063,0.00012293617,0.0004369109,0.0011253431,0.00050583127,0.031185647,0.00033129327,0.00060313975,0.029289622],"study_design_scores_gemma":[0.000019796718,0.00010850288,0.9890548,0.000015458936,0.00006829695,0.0003646193,0.00036849923,0.0009894088,0.0055530933,0.00012302304,0.003322342,0.000012219595],"about_ca_topic_score_codex":0.0063706385,"about_ca_topic_score_gemma":0.015326728,"teacher_disagreement_score":0.0063706385,"about_ca_system_score_codex":0.00042709595,"about_ca_system_score_gemma":0.0007841745,"threshold_uncertainty_score":0.0126671195},"labels":[],"label_agreement":null},{"id":"W2950552986","doi":"10.1088/0004-637x/789/1/49","title":"THREE-DIMENSIONAL SIMULATIONS OF THE NON-THERMAL BROADBAND EMISSION FROM YOUNG SUPERNOVA REMNANTS INCLUDING EFFICIENT PARTICLE ACCELERATION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Agence Nationale de la Recherche","keywords":"Physics; Cosmic ray; Supernova; Particle acceleration; Electron; Astrophysics; Supernova remnant; Magnetic field; Acceleration; Shock (circulatory); Synchrotron; Computational physics; Range (aeronautics); Nuclear physics; Classical mechanics","score_opus":0.015996881731532894,"score_gpt":0.24106280082860998,"score_spread":0.22506591909707707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950552986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9645016,0.00032471836,0.01297602,0.0006121998,0.00012891079,0.00009231818,0.0021967867,0.00061307504,0.018554335],"genre_scores_gemma":[0.9863115,0.00024189382,0.007929842,0.00020830109,0.000050871473,0.00013938537,0.0018193052,0.00017431666,0.0031244836],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984515,0.000036590303,0.000009889954,0.000021204125,0.000032947497,0.000054223005],"domain_scores_gemma":[0.9990972,0.00046145046,0.00011229166,0.000042437772,0.00012435079,0.00016220905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003517894,0.0007417162,0.00061646255,0.00051640027,0.0006068572,0.0011139474,0.0010018952,0.0014998842,0.004475135],"category_scores_gemma":[0.001917519,0.0005065973,0.0009253532,0.00065831526,0.0009184285,0.00048793614,0.000879217,0.0010939519,0.0003247905],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000117174226,0.00009440028,0.0032514536,0.00003761016,0.00004617005,0.00014044663,0.000055853674,0.99203146,0.0009554002,0.0018573927,0.00045540745,0.0009571918],"study_design_scores_gemma":[0.00004739415,0.000026217405,0.0013378875,0.00000727025,0.000010082324,0.000013567779,0.000040519353,0.99725395,0.00023185629,0.00073479634,0.0002873525,0.000009062463],"about_ca_topic_score_codex":0.027713653,"about_ca_topic_score_gemma":0.0142363245,"teacher_disagreement_score":0.027713653,"about_ca_system_score_codex":0.0008952189,"about_ca_system_score_gemma":0.0009910294,"threshold_uncertainty_score":0.055104673},"labels":[],"label_agreement":null},{"id":"W2950619369","doi":"10.1088/0004-637x/749/1/32","title":"SWEEPING AWAY THE MYSTERIES OF DUSTY CONTINUOUS WINDS IN ACTIVE GALACTIC NUCLEI","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Western University","funders":"","keywords":"Active galactic nucleus; Torus; Spectral line; Kinetic energy; Spectral shape analysis; Luminosity; Acceleration; Radiation; Sky","score_opus":0.014511628203908682,"score_gpt":0.2387807296429244,"score_spread":0.2242691014390157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950619369","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96311903,0.0038659107,0.023527693,0.0032558984,0.00006999765,0.000006491025,0.00017997445,0.000116668605,0.005858354],"genre_scores_gemma":[0.9970324,0.0008990452,0.0013833388,0.00013473026,0.00004028144,0.0000030499755,0.000033948203,0.000018361388,0.00045483897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990106,0.000037706992,0.0000034404964,0.000028100134,0.000019341935,0.000010407239],"domain_scores_gemma":[0.9994609,0.0002647278,0.00010149008,0.000078599085,0.00003641315,0.00005784115],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044106581,0.0002189841,0.00024704906,0.00017311049,0.00038536056,0.0012840781,0.000672647,0.00071074214,0.0009274535],"category_scores_gemma":[0.0022553727,0.00020495588,0.00020758479,0.00019878717,0.0015135392,0.0024991848,0.00044886314,0.0006337059,0.00017329148],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047973264,0.00015883608,0.33048722,0.000421116,0.00024853952,0.0012717015,0.0035830175,0.3027917,0.019556947,0.26081377,0.004985843,0.07520161],"study_design_scores_gemma":[0.000060728664,0.00013600299,0.13445672,0.00022053433,0.000049566755,0.0005767638,0.0035850268,0.32838282,0.0023440938,0.51671064,0.013378948,0.00009813573],"about_ca_topic_score_codex":0.0034221706,"about_ca_topic_score_gemma":0.003938171,"teacher_disagreement_score":0.0034221706,"about_ca_system_score_codex":0.0003991389,"about_ca_system_score_gemma":0.00022748759,"threshold_uncertainty_score":0.006804526},"labels":[],"label_agreement":null},{"id":"W2950720496","doi":"10.1088/0004-637x/736/1/57","title":"DISCOVERY OF A RADIO-SELECTED<i>z</i>∼ 6 QUASAR","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Quasar; Sky; Context (archaeology); Telescope; OVV quasar; Large Synoptic Survey Telescope; Red shift","score_opus":0.00956306729087745,"score_gpt":0.1976724841656891,"score_spread":0.18810941687481167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950720496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9923419,0.00029671856,0.0008488762,0.00028292026,0.000037525784,0.000014125024,0.00026151826,0.000111248555,0.0058052028],"genre_scores_gemma":[0.9971819,0.00009824908,0.0010724067,0.000256691,0.00006593263,0.000005898735,0.00040854825,0.000010456669,0.00090001296],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998739,0.00000434726,0.0000054305683,0.000032776577,0.0000304243,0.000053095093],"domain_scores_gemma":[0.99944276,0.00004893634,0.00016928109,0.000037051144,0.00005749988,0.00024438274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029469712,0.0002561236,0.00032245528,0.00069263345,0.00047538712,0.0011309254,0.0004455997,0.00049356004,0.00179545],"category_scores_gemma":[0.0003759859,0.00022027931,0.00020417821,0.00034032503,0.00043897482,0.00033599176,0.0006885864,0.00057224435,0.00066115847],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051149155,0.00034510897,0.7294899,0.0001428747,0.00009612915,0.007394606,0.0012305704,0.00024289741,0.21802156,0.0032013867,0.0033703647,0.03595309],"study_design_scores_gemma":[0.000036412912,0.0005367994,0.97483385,0.000016479116,0.00004710545,0.005743985,0.00023140897,0.0002738166,0.007326085,0.00043948813,0.010494592,0.000019945019],"about_ca_topic_score_codex":0.0009593437,"about_ca_topic_score_gemma":0.0018168982,"teacher_disagreement_score":0.00179545,"about_ca_system_score_codex":0.00019263667,"about_ca_system_score_gemma":0.00010566166,"threshold_uncertainty_score":0.00600636},"labels":[],"label_agreement":null},{"id":"W2950898382","doi":"10.3847/1538-4357/ab1e4d","title":"The Fate of Binaries in the Galactic Center: The Mundane and the Exotic","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Galactic Center; Astronomy; Astrophysics; Center (category theory); Astrobiology; Stars","score_opus":0.00950488968880835,"score_gpt":0.20990194288939673,"score_spread":0.20039705320058837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2950898382","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978661,0.00030893684,0.000077260804,0.000081193415,0.000005405953,0.0000016306071,0.000039473118,0.0000025193656,0.0016175266],"genre_scores_gemma":[0.9997328,0.00006222037,0.000022479067,0.000011698579,0.000002633103,3.59705e-7,0.000043303473,9.8791e-7,0.0001234147],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990404,0.000013124492,0.000005229242,0.00002386657,0.000019342397,0.000034383793],"domain_scores_gemma":[0.999519,0.000029932562,0.00017074679,0.00004578636,0.000032718544,0.00020177262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002790768,0.00013229252,0.00019936153,0.00049795315,0.0010030278,0.0011742942,0.00022823125,0.00033867193,0.0022335928],"category_scores_gemma":[0.000703324,0.00007280572,0.000088092245,0.00040694416,0.0007644646,0.00073939364,0.0012737396,0.00035436422,0.00030780557],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034865894,0.000075578595,0.9750313,0.000022738757,0.00003169353,0.0008498029,0.0007064442,0.0005267609,0.0036075262,0.006983764,0.0005502119,0.0112654595],"study_design_scores_gemma":[0.000019694777,0.00021299692,0.9666563,0.00006236625,0.00002687063,0.003099554,0.004125119,0.005019188,0.002207614,0.0107380375,0.0078005306,0.000031581007],"about_ca_topic_score_codex":0.0032564928,"about_ca_topic_score_gemma":0.0038223607,"teacher_disagreement_score":0.0032564928,"about_ca_system_score_codex":0.0005504311,"about_ca_system_score_gemma":0.00019332263,"threshold_uncertainty_score":0.007472098},"labels":[],"label_agreement":null},{"id":"W2951156939","doi":"10.1088/0004-637x/706/1/l164","title":"PROBING THE EPOCH OF REIONIZATION WITH THE Lyα FOREST AT <i>z</i> ∼ 4-5","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; Quasar; Flux (metallurgy); Redshift; Lyman-alpha forest; Intergalactic medium; Epoch (astronomy); Spectral density; Intergalactic travel","score_opus":0.005012524945483548,"score_gpt":0.18813961832791737,"score_spread":0.18312709338243383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951156939","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968671,0.0000823209,0.00042830862,0.000030966374,0.000001201299,0.0000029107957,0.00012373597,0.000016921436,0.0024465541],"genre_scores_gemma":[0.9993801,0.000033324657,0.00026678506,0.000009111766,0.0000017326857,0.0000010596546,0.00008236008,0.0000020840528,0.00022321063],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999602,0.0000046741375,0.0000012384025,0.000008423813,0.000005788127,0.000019705127],"domain_scores_gemma":[0.999676,0.000050036037,0.00016529782,0.000019735648,0.000025151303,0.000063840336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015559954,0.00015344062,0.00007976575,0.0006278645,0.00020726283,0.00043734172,0.00016991355,0.00018861788,0.0015460309],"category_scores_gemma":[0.00046930986,0.00010193897,0.000121338315,0.0003180705,0.00017458711,0.00042467017,0.0003334682,0.0003141482,0.00023112954],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020790573,0.000039635896,0.9396364,0.000017456608,0.000040059836,0.0001914961,0.00038068646,0.0003977959,0.043889392,0.0015902763,0.0002813595,0.013327455],"study_design_scores_gemma":[0.0000020607106,0.00002704743,0.9948331,0.0000040399427,0.000009830284,0.000099372824,0.00011325551,0.00035580905,0.003740945,0.00028492208,0.0005270531,0.0000025586473],"about_ca_topic_score_codex":0.0026349325,"about_ca_topic_score_gemma":0.00462965,"teacher_disagreement_score":0.0026349325,"about_ca_system_score_codex":0.00024912276,"about_ca_system_score_gemma":0.00006869235,"threshold_uncertainty_score":0.0052391887},"labels":[],"label_agreement":null},{"id":"W2951208331","doi":"10.1088/0004-637x/737/2/99","title":"A VERY DEEP<i>CHANDRA</i>OBSERVATION OF A2052: BUBBLES, SHOCKS, AND SLOSHING","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":125,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Perimeter Institute","funders":"","keywords":"Spiral (railway); Brightness; Bubble; Slosh dynamics; Spiral galaxy; Surface brightness; Brightness temperature","score_opus":0.024557277554147817,"score_gpt":0.21603134552261957,"score_spread":0.19147406796847175,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951208331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9926745,0.00022629854,0.00053075916,0.000093455936,0.000020823663,0.000020984544,0.0015834052,0.00015661793,0.0046930793],"genre_scores_gemma":[0.9963385,0.000063934625,0.0010835342,0.00012112416,0.000028342503,0.000010541927,0.0016516617,0.000016411565,0.00068594783],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999356,0.0000028066354,0.000001975372,0.000016618167,0.000015237157,0.00002770354],"domain_scores_gemma":[0.9998436,0.000011955169,0.00003094819,0.000015725056,0.000009513437,0.00008820348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007797506,0.00031543573,0.00022506155,0.00071345497,0.000697546,0.00049388834,0.00024495178,0.00035763741,0.0017439297],"category_scores_gemma":[0.00012025556,0.00018301915,0.0002363996,0.00047182155,0.00020908315,0.00019615085,0.00047843726,0.00043519287,0.0003270828],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019418811,0.0004931417,0.2652234,0.00030101667,0.00029397293,0.0077792415,0.00095596316,0.0010158643,0.68634945,0.001035269,0.007904859,0.026706012],"study_design_scores_gemma":[0.0000432154,0.00026459442,0.9783547,0.000019431896,0.000039917086,0.0021967124,0.00019074968,0.0007277031,0.012411918,0.00020252787,0.0055122077,0.00003627297],"about_ca_topic_score_codex":0.005263603,"about_ca_topic_score_gemma":0.016460184,"teacher_disagreement_score":0.005263603,"about_ca_system_score_codex":0.00030176897,"about_ca_system_score_gemma":0.00019963393,"threshold_uncertainty_score":0.01046592},"labels":[],"label_agreement":null},{"id":"W2951230111","doi":"10.1088/0004-637x/719/1/685","title":"NEW RESULTS FROM THE MAGELLAN IMACS SPECTROSCOPIC Lyα SURVEY: NICMOS OBSERVATIONS OF Lyα EMITTERS AT<i>z</i>= 5.7","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Redshift; Astrophysics; Rest frame; Galaxy; Angstrom; Astronomy; Spectroscopy; Narrowband; Doubly ionized oxygen; Emission spectrum; Spectral line; Optics; Chemistry","score_opus":0.01470308716637778,"score_gpt":0.22202484106338938,"score_spread":0.2073217538970116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951230111","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93664485,0.0007621882,0.002655006,0.00034196535,0.000070431925,0.00005931969,0.026345905,0.00045081135,0.032669425],"genre_scores_gemma":[0.9260708,0.0007377342,0.011703053,0.00045017592,0.00017872146,0.00007898569,0.055277895,0.00018533824,0.0053172866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994992,0.00003893083,0.000045034027,0.00012553156,0.0002252307,0.00006612588],"domain_scores_gemma":[0.9981375,0.00013379513,0.0006127249,0.00037699947,0.00045177096,0.00028708944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006485896,0.0004458306,0.00023696694,0.0029013585,0.00039647068,0.0010582433,0.00046467083,0.00028920828,0.0020184768],"category_scores_gemma":[0.0012894382,0.00021818007,0.00028988213,0.0015491843,0.00027372665,0.00046303612,0.0013590092,0.00033971368,0.0010596965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003373047,0.00011631065,0.93460125,0.00020016552,0.00013120893,0.00050625677,0.00082395354,0.0005891853,0.0218141,0.001198663,0.011167063,0.028514553],"study_design_scores_gemma":[0.0000075873786,0.000021176227,0.9825952,0.000025274338,0.000049883853,0.0004735661,0.00024509826,0.00049337896,0.00278654,0.00016661157,0.013117964,0.000017709672],"about_ca_topic_score_codex":0.014458693,"about_ca_topic_score_gemma":0.052227635,"teacher_disagreement_score":0.014458693,"about_ca_system_score_codex":0.0006039557,"about_ca_system_score_gemma":0.0003337821,"threshold_uncertainty_score":0.028749049},"labels":[],"label_agreement":null},{"id":"W2951299963","doi":"10.1088/0004-637x/704/1/715","title":"VARIABLE ACCRETION IN THE EMBEDDED PHASE OF STAR FORMATION","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Accretion (finance); Young stellar object; Star formation; T Tauri star; Stellar mass; Protostar; Ophiuchus; Intermediate polar; Stellar evolution","score_opus":0.014385639363268803,"score_gpt":0.2746508637967597,"score_spread":0.26026522443349087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951299963","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977303,0.000046709007,0.0012921338,0.0000076988945,0.0000025546517,0.000005892294,0.000046903984,0.0000120136665,0.0008558905],"genre_scores_gemma":[0.99925274,0.000040161893,0.00044767527,0.0000050909875,0.0000027348945,0.0000051341617,0.00008075826,0.0000046275654,0.00016105532],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999372,0.000011841575,0.0000047348385,0.000018771067,0.000011783097,0.000015626512],"domain_scores_gemma":[0.99976426,0.000069980066,0.00007106054,0.000032033833,0.000024072679,0.000038636565],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012830502,0.00033446634,0.00027182786,0.00020327263,0.0002361358,0.0007494818,0.0005266289,0.00030263592,0.0005714766],"category_scores_gemma":[0.0012910567,0.00013384472,0.0003372263,0.00019702058,0.00034976474,0.0004519295,0.0005075548,0.0002709223,0.00009378935],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002688794,0.00024433815,0.15753238,0.00007781816,0.00013251335,0.00091853493,0.00036611618,0.7965142,0.024676373,0.011112166,0.00019803588,0.007958728],"study_design_scores_gemma":[0.00008418893,0.00020988754,0.06491958,0.000018729224,0.000044648616,0.00027414598,0.00014152999,0.92090255,0.0071665696,0.005334071,0.0008769175,0.000027162178],"about_ca_topic_score_codex":0.0034585309,"about_ca_topic_score_gemma":0.0018275018,"teacher_disagreement_score":0.0034585309,"about_ca_system_score_codex":0.0004269471,"about_ca_system_score_gemma":0.00037044467,"threshold_uncertainty_score":0.0068768263},"labels":[],"label_agreement":null},{"id":"W2951370613","doi":"10.3847/1538-4357/aad3d2","title":"The Next Generation Virgo Cluster Survey (NGVS). XXXI. The Kinematics of Intracluster Globular Clusters in the Core of the Virgo Cluster","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Australian Astronomical Optics-Macquarie; Institut national des sciences de l'Univers; Comisión Nacional de Investigación Científica y Tecnológica; Canadian Space Agency; Centro de Astrofísica y Tecnologías Afines; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; National Natural Science Foundation of China; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Chinese Academy of Sciences South America Center for Astronomy; Smithsonian Institution; National Science Foundation","keywords":"Virgo Cluster; Physics; Globular cluster; Astrophysics; Galaxy; Population; Astronomy; Velocity dispersion; Galaxy cluster; Halo; Star cluster; Cluster (spacecraft)","score_opus":0.026332183840906968,"score_gpt":0.24397856717286634,"score_spread":0.21764638333195938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951370613","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98288673,0.00033916876,0.00034537655,0.000059067388,0.000006714255,0.00002034547,0.012767223,0.00006919145,0.0035061862],"genre_scores_gemma":[0.9782574,0.0001542391,0.0007770781,0.000045647117,0.0000061527244,0.000014680877,0.019183759,0.000013179258,0.0015478824],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999298,0.000009272878,0.0000035495202,0.000019256464,0.000019466699,0.000018666424],"domain_scores_gemma":[0.99982005,0.000015981152,0.00005345753,0.00002298327,0.000036503436,0.000051034738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014077472,0.00008654106,0.000091878086,0.001080639,0.00015825941,0.00023747742,0.0001529237,0.00012251723,0.0014128253],"category_scores_gemma":[0.00030111603,0.000052580577,0.00011723014,0.00062282826,0.00008167931,0.000106071726,0.00034583348,0.000083577936,0.00045820695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052249543,0.000014590055,0.9763476,0.00002914689,0.00004466375,0.000052707575,0.00013348956,0.00026696193,0.0050099427,0.00021655265,0.0029283762,0.014903659],"study_design_scores_gemma":[0.0000013694946,0.000004791417,0.9973271,0.0000042367897,0.000005674049,0.0000334493,0.000037880945,0.0002750052,0.00028245078,0.000030363568,0.0019965733,0.0000011023442],"about_ca_topic_score_codex":0.023679579,"about_ca_topic_score_gemma":0.039981913,"teacher_disagreement_score":0.023679579,"about_ca_system_score_codex":0.00034277103,"about_ca_system_score_gemma":0.0001545522,"threshold_uncertainty_score":0.047083497},"labels":[],"label_agreement":null},{"id":"W2951388598","doi":"10.1088/0004-637x/783/2/73","title":"ACTIVE GALACTIC NUCLEUS AND QUASAR SCIENCE WITH APERTURE MASKING INTERFEROMETRY ON THE<i>JAMES WEBB SPACE TELESCOPE</i>","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Active galactic nucleus; James Webb Space Telescope; Supermassive black hole; Quasar; Galaxy; Angular resolution (graph drawing); Binary number; Accretion (finance); Point source","score_opus":0.005524065673684185,"score_gpt":0.20046546768074294,"score_spread":0.19494140200705876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951388598","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92459387,0.00033018392,0.053773317,0.00049789477,0.000065742446,0.000072430725,0.0017744412,0.0015531334,0.017339109],"genre_scores_gemma":[0.9680826,0.00011313465,0.029749604,0.00006611514,0.00002632428,0.000028478593,0.0011299534,0.00008170518,0.00072207896],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999082,0.000020697018,0.000003324189,0.000020119078,0.000036027013,0.000011576078],"domain_scores_gemma":[0.99984694,0.00003960915,0.000026538035,0.000028528693,0.000024721947,0.000033634933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035361352,0.00026863776,0.00014185121,0.00022224359,0.00018696627,0.00039562403,0.00044487117,0.00024020344,0.001095391],"category_scores_gemma":[0.000513037,0.00012627538,0.0002967338,0.0002590456,0.00021368453,0.00030444664,0.00030790947,0.00019390932,0.00021473905],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041696584,0.00016782623,0.10710794,0.00010020885,0.00020921837,0.00033629217,0.000170204,0.78862745,0.046653673,0.009244878,0.008135761,0.038829584],"study_design_scores_gemma":[0.00004648898,0.000111701156,0.06694953,0.000017022623,0.00003195732,0.00009217819,0.00003175323,0.92127156,0.0036332735,0.0035182487,0.0042738263,0.000022421722],"about_ca_topic_score_codex":0.014338527,"about_ca_topic_score_gemma":0.014188203,"teacher_disagreement_score":0.014338527,"about_ca_system_score_codex":0.00038345167,"about_ca_system_score_gemma":0.00034953587,"threshold_uncertainty_score":0.028510153},"labels":[],"label_agreement":null},{"id":"W2951538781","doi":"10.3847/1538-4357/ab77ac","title":"Chromium Nucleosynthesis and Silicon–Carbon Shell Mergers in Massive Stars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Los Alamos National Laboratory; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; Magyar Tudományos Akadémia; Compute Canada; University of Hull; Laboratory Directed Research and Development; U.S. Department of Energy; National Science Foundation","keywords":"Nucleosynthesis; Stars; Metallicity; Supernova; Milky Way; Stellar evolution; Stellar nucleosynthesis; Shell (structure)","score_opus":0.009977110549802264,"score_gpt":0.20660886298820283,"score_spread":0.19663175243840056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951538781","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99785906,0.000052187097,0.00084900955,0.00003519295,0.000003847336,0.0000048848337,0.00022667332,0.000037940896,0.00093113264],"genre_scores_gemma":[0.9990483,0.000027855342,0.00041779788,0.000007964228,0.0000024339263,0.000006035238,0.00023216738,0.000013626766,0.0002439106],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999274,0.000021435097,0.00000408128,0.00001821152,0.0000115011635,0.000017425282],"domain_scores_gemma":[0.9997683,0.00009645589,0.00004713495,0.000024976545,0.00002482073,0.000038334878],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003171164,0.0006265918,0.0003218002,0.00049076194,0.00033488337,0.0006623341,0.00054313,0.0006786386,0.001086336],"category_scores_gemma":[0.00087061414,0.00029962746,0.0008306618,0.0003326157,0.00037466007,0.00031789162,0.00043814955,0.000320433,0.00021024683],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018099119,0.00007008003,0.056714807,0.000021943306,0.00014349994,0.00019758716,0.000042981796,0.9346595,0.005039638,0.0013659203,0.00016319382,0.0013998386],"study_design_scores_gemma":[0.000049391776,0.00010675208,0.024056787,0.000005107955,0.000042839332,0.00006126966,0.00004360996,0.9710745,0.00339706,0.0007297651,0.00041741476,0.000015376705],"about_ca_topic_score_codex":0.018229747,"about_ca_topic_score_gemma":0.0075009335,"teacher_disagreement_score":0.018229747,"about_ca_system_score_codex":0.00084880064,"about_ca_system_score_gemma":0.0002481234,"threshold_uncertainty_score":0.036247313},"labels":[],"label_agreement":null},{"id":"W2951563203","doi":"10.1088/0004-637x/740/2/52","title":"ARE THERE ECHOES FROM THE PRE-BIG-BANG UNIVERSE? A SEARCH FOR LOW-VARIANCE CIRCLES IN THE COSMIC MICROWAVE BACKGROUND SKY","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Sky; Cosmology; Cosmic background radiation; Cosmic variance; Anisotropy; Noise (video); Gaussian","score_opus":0.02911012324142248,"score_gpt":0.2566856129289169,"score_spread":0.22757548968749441,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951563203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9946249,0.00017185575,0.0036430974,0.0002021918,0.000007220569,0.000003920562,0.000046604408,0.000033895274,0.0012662159],"genre_scores_gemma":[0.9989273,0.000050215604,0.0008554509,0.000024595243,0.000013225906,0.0000012760751,0.000038565875,0.000007804974,0.000081561775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982834,0.000043116353,0.000007741854,0.00005803096,0.000039392973,0.000023256334],"domain_scores_gemma":[0.9949588,0.0027381699,0.0010322399,0.0006007835,0.00030320036,0.0003669029],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007415129,0.00015768476,0.00026513953,0.0006525068,0.00041502883,0.0015404101,0.00057582365,0.0006656506,0.0014737464],"category_scores_gemma":[0.0064615337,0.0002393361,0.00017332022,0.0006218988,0.0010028133,0.001494962,0.00046628746,0.00036897248,0.00020080514],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019383548,0.00017622768,0.773426,0.00027566345,0.00032688517,0.0023158893,0.0048286226,0.008320652,0.05520593,0.06077564,0.0021310328,0.09027916],"study_design_scores_gemma":[0.00012226313,0.00025118582,0.8455533,0.00006661426,0.00022388747,0.0026667288,0.0029969502,0.06976821,0.015105512,0.058052007,0.005054694,0.00013863109],"about_ca_topic_score_codex":0.000578998,"about_ca_topic_score_gemma":0.00054561923,"teacher_disagreement_score":0.0015404101,"about_ca_system_score_codex":0.00020665485,"about_ca_system_score_gemma":0.00008934355,"threshold_uncertainty_score":0.004930198},"labels":[],"label_agreement":null},{"id":"W2951789435","doi":"10.1088/0004-637x/695/1/l45","title":"THREE-DIMENSIONAL GENUS TOPOLOGY OF LUMINOUS RED GALAXIES","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Topology (electrical circuits); Physics; Measure (data warehouse); Smoothing; Galaxy; Genus; Astrophysics; Mathematics; Computer science; Statistics; Biology; Combinatorics","score_opus":0.008088264224276375,"score_gpt":0.21508736845883766,"score_spread":0.20699910423456128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951789435","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99835,0.000029871364,0.0008938961,0.000020375142,6.865661e-7,0.0000013552743,0.00015342954,0.000034156525,0.0005161223],"genre_scores_gemma":[0.99911517,0.000016070506,0.0005375156,0.0000027918336,0.0000015234915,0.0000013518165,0.0002757106,0.000006974291,0.00004285358],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998605,0.000045630488,0.0000068866516,0.000030413103,0.000027518065,0.000028994269],"domain_scores_gemma":[0.9982613,0.00048434013,0.00058504334,0.00022547536,0.0001685881,0.00027532238],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003979721,0.0002000438,0.00017427842,0.0022153913,0.00028264322,0.0007369126,0.00020172761,0.0002275366,0.0006196098],"category_scores_gemma":[0.002572163,0.00020495158,0.0002709352,0.0009234943,0.0006120256,0.0005296978,0.000604453,0.00020786368,0.00009258979],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038663324,0.000047332436,0.8609917,0.00006221417,0.00014959242,0.00031293425,0.0012204048,0.08096676,0.024024172,0.013230235,0.0008111646,0.017796874],"study_design_scores_gemma":[0.000012059837,0.00004149178,0.8821068,0.000012275631,0.000023257919,0.00021960752,0.00026061063,0.10826456,0.0030369447,0.00524747,0.00074073946,0.00003426196],"about_ca_topic_score_codex":0.003013896,"about_ca_topic_score_gemma":0.002786654,"teacher_disagreement_score":0.003013896,"about_ca_system_score_codex":0.000504174,"about_ca_system_score_gemma":0.00010927243,"threshold_uncertainty_score":0.0059927106},"labels":[],"label_agreement":null},{"id":"W2951878034","doi":"10.3847/1538-4357/ab0e7f","title":"The MESAS Project: Long-wavelength Follow-up Observations of Sirius A","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University; University of British Columbia","funders":"","keywords":"Sirius; Stars; Stellar atmosphere; Millimeter; Atmosphere (unit); Ejecta; Stellar evolution","score_opus":0.022809595597595003,"score_gpt":0.25370088524929535,"score_spread":0.23089128965170036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951878034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.983748,0.0001832627,0.0017021184,0.000109853165,0.000024647581,0.00002403111,0.0070908885,0.0003699146,0.0067472383],"genre_scores_gemma":[0.9805582,0.00013284877,0.00667861,0.00010196209,0.00005228286,0.000026969743,0.010114885,0.00009356104,0.0022407286],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998653,0.000018501114,0.0000050396934,0.000057879122,0.000034791236,0.000018438865],"domain_scores_gemma":[0.9995054,0.000034646422,0.00014626404,0.000094655436,0.000089810994,0.00012909345],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000513776,0.0002531226,0.00019455398,0.00080360373,0.00040961237,0.00042473074,0.00032357496,0.000210393,0.0015194165],"category_scores_gemma":[0.00028438127,0.00018591688,0.00033527822,0.00038459848,0.00015202824,0.000316794,0.00062920334,0.00035139103,0.00087164517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009733582,0.00033568067,0.7879002,0.00012120839,0.00045967888,0.00054828555,0.00063943974,0.0023042706,0.15470305,0.0015049818,0.012682467,0.03782734],"study_design_scores_gemma":[0.00003631501,0.00011273929,0.9774311,0.000013612533,0.000039848765,0.00014021495,0.00014376872,0.0035402973,0.0062015695,0.00031300975,0.012015339,0.0000122661795],"about_ca_topic_score_codex":0.0028218077,"about_ca_topic_score_gemma":0.0076862397,"teacher_disagreement_score":0.0028218077,"about_ca_system_score_codex":0.00022273873,"about_ca_system_score_gemma":0.00019985715,"threshold_uncertainty_score":0.005610764},"labels":[],"label_agreement":null},{"id":"W2951948035","doi":"10.3847/1538-4357/ab11d0","title":"Detection of a White Dwarf Companion to a Blue Straggler Star in the Outskirts of Globular Cluster NGC 5466 with the Ultraviolet Imaging Telescope (UVIT)","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Calgary","funders":"","keywords":"Globular cluster; White dwarf; RADIUS; Proper motion; Star cluster; Blue straggler; Spectral energy distribution; Telescope; Open cluster","score_opus":0.005124028059854184,"score_gpt":0.20459258261701044,"score_spread":0.19946855455715626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951948035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996948,0.000015375823,0.000053934054,0.000005076824,0.0000013157327,0.0000013920862,0.00004884982,0.0000070521437,0.00017237169],"genre_scores_gemma":[0.9995901,0.000012647375,0.00015244368,0.0000067953697,0.0000024564488,8.6933375e-7,0.0000958198,0.0000018823006,0.00013707226],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999044,0.0000056013923,0.000006568619,0.00002851015,0.000030732303,0.000024230934],"domain_scores_gemma":[0.999726,0.000020961188,0.00009270701,0.000036745954,0.000029813455,0.00009371272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001154603,0.00027935978,0.00020045506,0.0007514116,0.0006272436,0.00032957,0.00026715887,0.00024404172,0.00077269686],"category_scores_gemma":[0.00025838823,0.00013442988,0.0001490987,0.00049621635,0.00027860544,0.00014666967,0.00039637164,0.00017934781,0.00020308066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013056441,0.000039123814,0.93290263,0.00001540309,0.000032891745,0.0016935564,0.00048207128,0.00019217568,0.06053591,0.000085157,0.00021267364,0.0036779372],"study_design_scores_gemma":[0.0000033891836,0.00008450276,0.99328655,0.0000033475362,0.000019264184,0.0010303962,0.000233137,0.00030702262,0.004443908,0.000026664682,0.00055644056,0.0000054282323],"about_ca_topic_score_codex":0.01107827,"about_ca_topic_score_gemma":0.021509405,"teacher_disagreement_score":0.01107827,"about_ca_system_score_codex":0.00033410083,"about_ca_system_score_gemma":0.00011540582,"threshold_uncertainty_score":0.022027552},"labels":[],"label_agreement":null},{"id":"W2951973311","doi":"10.1088/0004-637x/740/2/51","title":"AVERAGE HEATING RATE OF HOT ATMOSPHERES IN DISTANT CLUSTERS BY RADIO ACTIVE GALACTIC NUCLEUS: EVIDENCE FOR CONTINUOUS ACTIVE GALACTIC NUCLEUS HEATING","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Active galactic nucleus; Radio galaxy; Galaxy cluster; Redshift; Cluster (spacecraft); RADIUS; Luminosity; Intracluster medium","score_opus":0.0175959276954259,"score_gpt":0.24047069562499082,"score_spread":0.22287476792956493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2951973311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997155,0.00003349847,0.00003917347,0.0000024311448,4.001453e-7,6.156383e-7,0.000049942853,0.000005487072,0.00015292178],"genre_scores_gemma":[0.9997379,0.0000135743085,0.00004407263,0.0000015314092,0.0000017852751,7.160061e-7,0.00013910196,0.0000025814636,0.000058747228],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.000011485139,0.0000069197067,0.000048608672,0.000029233637,0.000025998605],"domain_scores_gemma":[0.9990621,0.00020728246,0.00028712198,0.0001420239,0.00009728466,0.00020414437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017961873,0.00013157293,0.00018244034,0.0006717044,0.00022099244,0.00041926905,0.00024027786,0.0001775588,0.0010288067],"category_scores_gemma":[0.0010292085,0.00016355996,0.00021085491,0.00038835552,0.00025967913,0.00025380187,0.00043990166,0.00014768657,0.0001939622],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009180875,0.0000105483305,0.98724025,0.000010292154,0.00006265496,0.000071536946,0.00016059262,0.00095963717,0.009465274,0.000054493234,0.000052460335,0.001820402],"study_design_scores_gemma":[0.000001040842,0.00001401919,0.9991466,4.127123e-7,0.0000065672475,0.000049961298,0.00003108517,0.0003635167,0.00033766712,0.000013214296,0.00003428309,0.0000016443254],"about_ca_topic_score_codex":0.0033504092,"about_ca_topic_score_gemma":0.0031510794,"teacher_disagreement_score":0.0033504092,"about_ca_system_score_codex":0.00019523656,"about_ca_system_score_gemma":0.00006936985,"threshold_uncertainty_score":0.0066618323},"labels":[],"label_agreement":null},{"id":"W2952198119","doi":"10.1086/590369","title":"<i>MOST</i>Detects SPBe Pulsations in HD 127756 and HD 217543: Asteroseismic Rotation Rates Independent of<i>v</i> sin <i>i</i>","year":2008,"lang":"he","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Université du Québec à Montréal; Université de Montréal; Saint Mary's University; St. Mary's University; University of British Columbia","funders":"","keywords":"Stars; Physics; Astrophysics; Photometry (optics); Opacity; Rotation (mathematics); Astronomy; Optics; Geometry","score_opus":0.013850205511055008,"score_gpt":0.22564156943100794,"score_spread":0.21179136391995293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952198119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963921,0.00006935581,0.0003396154,0.00002109956,0.000002631743,0.000002609868,0.0007647175,0.00004277539,0.002365096],"genre_scores_gemma":[0.9981117,0.000023964525,0.00051322725,0.0000072887337,0.0000034511036,0.0000025598017,0.0011648525,0.0000057408215,0.00016733262],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992824,0.000005401952,0.000005054682,0.000022112883,0.000021411579,0.000017834476],"domain_scores_gemma":[0.9998053,0.000030898525,0.000069160626,0.000024362873,0.000022632808,0.000047736416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010724735,0.00015472973,0.0001558453,0.00076163566,0.00027748305,0.00029623686,0.0001571002,0.00020094514,0.0011774017],"category_scores_gemma":[0.00035504205,0.000087435605,0.00013601714,0.000505353,0.00017817937,0.00016094325,0.0002836123,0.00012286365,0.00023545505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023293655,0.000019573505,0.923997,0.000040171417,0.00004969192,0.00012795068,0.00021313292,0.0005104404,0.05646474,0.00028890342,0.0009463279,0.017109197],"study_design_scores_gemma":[0.0000038277603,0.000024411014,0.9921874,0.0000041944486,0.000014175328,0.00026545723,0.000055382174,0.0006431022,0.005939805,0.00006192556,0.00079600874,0.000004431379],"about_ca_topic_score_codex":0.0047974773,"about_ca_topic_score_gemma":0.012618845,"teacher_disagreement_score":0.0047974773,"about_ca_system_score_codex":0.00024232293,"about_ca_system_score_gemma":0.000094506315,"threshold_uncertainty_score":0.009539127},"labels":[],"label_agreement":null},{"id":"W2952309280","doi":"10.1086/342091","title":"Discovery of High-Latitude CO in an H [CSC]i[/CSC] Supershell in NGC 5775","year":2002,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Toronto","funders":"","keywords":"Line (geometry); Kinetic energy; Latitude; Excited state; Cosmic ray; Molecular cloud","score_opus":0.010263749713517767,"score_gpt":0.21544835973390777,"score_spread":0.20518461002039,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952309280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990397,0.00006971992,0.0000798814,0.0000067196834,0.0000025675556,0.0000025350157,0.000041458567,0.000006332589,0.00075106893],"genre_scores_gemma":[0.99953127,0.000024215704,0.00013798843,0.000009806598,0.0000025820034,0.0000016391314,0.00010045662,0.0000016418161,0.00019044057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999144,0.0000026150312,0.0000035501255,0.000018054818,0.000029296249,0.00003202914],"domain_scores_gemma":[0.9998739,0.000007425333,0.000034138848,0.00001210374,0.00002314166,0.000049385682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006687098,0.00018776681,0.00015201562,0.00081952946,0.00072232925,0.000571852,0.00038856603,0.00029571878,0.00059089094],"category_scores_gemma":[0.00016706501,0.00014108367,0.00016169992,0.0003960406,0.00030849772,0.00012995572,0.00039771988,0.00013615728,0.0002139157],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022226191,0.00005255327,0.5389897,0.00004569323,0.00013103339,0.0052170963,0.0014237321,0.00042787878,0.4410962,0.0007852004,0.00047223084,0.0111364415],"study_design_scores_gemma":[0.0000051480038,0.0000883655,0.9835565,0.000011578183,0.0000374509,0.0012605565,0.00056586025,0.00053738547,0.011868345,0.00008884174,0.0019688508,0.000011099029],"about_ca_topic_score_codex":0.028634196,"about_ca_topic_score_gemma":0.04775405,"teacher_disagreement_score":0.028634196,"about_ca_system_score_codex":0.0005515608,"about_ca_system_score_gemma":0.0001987849,"threshold_uncertainty_score":0.056935012},"labels":[],"label_agreement":null},{"id":"W2952323009","doi":"10.1086/421380","title":"The Black Hole Mass versus Velocity Dispersion Relation in QSOs/Active Galactic Nuclei: Observational Appearance and Black Hole Growth","year":2004,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Velocity dispersion; Luminosity; Black hole (networking); Accretion (finance); Galaxy; Dispersion relation; Supermassive black hole; Dispersion (optics); Eddington luminosity","score_opus":0.013286317164321748,"score_gpt":0.21951182498472577,"score_spread":0.20622550782040402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952323009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99714786,0.00016605019,0.001818283,0.000038104194,0.000003119897,0.0000054952384,0.0001815256,0.000035164576,0.0006043786],"genre_scores_gemma":[0.99936336,0.00003307874,0.00041414,0.0000035251228,0.000001936747,0.0000025086706,0.00011759911,0.000004560365,0.000059316335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998915,0.000036438254,0.0000063278053,0.000034917364,0.00001478425,0.000015968217],"domain_scores_gemma":[0.9990565,0.000348188,0.00030034536,0.00010185102,0.000093250346,0.000099862766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051919674,0.0002167967,0.00018466251,0.0005124716,0.00020033507,0.00037965155,0.00032906077,0.0003449035,0.0006611018],"category_scores_gemma":[0.0022561958,0.00011907626,0.00027286285,0.0005121107,0.00040486417,0.00045567757,0.00030588708,0.00022951173,0.00012074563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016559166,0.00007006699,0.89405704,0.00007197376,0.00007438589,0.00032330948,0.00034864314,0.08008544,0.012017658,0.0044234972,0.0003981778,0.007964255],"study_design_scores_gemma":[0.00003715746,0.00010789586,0.7051222,0.000020227648,0.000047531466,0.0003095819,0.00016519288,0.28570828,0.004495582,0.0030491645,0.0009085643,0.0000286648],"about_ca_topic_score_codex":0.0075394553,"about_ca_topic_score_gemma":0.005196704,"teacher_disagreement_score":0.0075394553,"about_ca_system_score_codex":0.00049762125,"about_ca_system_score_gemma":0.00015953711,"threshold_uncertainty_score":0.014991105},"labels":[],"label_agreement":null},{"id":"W2952323727","doi":"10.1088/0004-637x/758/2/76","title":"PROBING THE INFLATON: SMALL-SCALE POWER SPECTRUM CONSTRAINTS FROM MEASUREMENTS OF THE COSMIC MICROWAVE BACKGROUND ENERGY SPECTRUM","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":276,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Cosmic microwave background; Spectral density; Inflation (cosmology); Amplitude; Primordial fluctuations; Dissipation; Limit (mathematics); Inflaton; Cosmic background radiation","score_opus":0.0166670393240951,"score_gpt":0.22602145120658632,"score_spread":0.2093544118824912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952323727","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9514396,0.00094568013,0.03783899,0.00030338007,0.000021899848,0.000011527484,0.0004457687,0.00030746308,0.008685701],"genre_scores_gemma":[0.99315614,0.00030552025,0.006076659,0.000025952977,0.000019568546,0.0000067820906,0.00019610439,0.00004433644,0.00016899823],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989367,0.000024325002,0.000004497223,0.00003772031,0.000022589436,0.000017105507],"domain_scores_gemma":[0.9993893,0.00029950708,0.00011713117,0.000114168,0.000032177788,0.00004777543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005167003,0.00056591554,0.00037229364,0.0004649127,0.00022368193,0.00069492543,0.00032625874,0.00040160277,0.0011470682],"category_scores_gemma":[0.0024859088,0.0003479961,0.00038861643,0.0004706218,0.00038196056,0.0007896089,0.0005593363,0.00056614674,0.00013566042],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014002571,0.0001878917,0.31890076,0.00070461375,0.00091708614,0.0012900492,0.00091008906,0.2384428,0.16756001,0.1656565,0.004049231,0.099980734],"study_design_scores_gemma":[0.00009955765,0.00015519328,0.36566612,0.00008847471,0.00015203634,0.0002949206,0.0001641511,0.5522348,0.027092041,0.048521318,0.0054120272,0.0001193413],"about_ca_topic_score_codex":0.0012805412,"about_ca_topic_score_gemma":0.0014368704,"teacher_disagreement_score":0.0012805412,"about_ca_system_score_codex":0.00022737091,"about_ca_system_score_gemma":0.00009743673,"threshold_uncertainty_score":0.0038372874},"labels":[],"label_agreement":null},{"id":"W2952332536","doi":"10.1086/317322","title":"MAXIMA-1: A Measurement of the Cosmic Microwave Background Anisotropy on Angular Scales of 10[arcmin]–5°","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":1294,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cosmic microwave background; Physics; Maxima; Anisotropy; Amplitude; Astrophysics; Bolometer; Photometer; Microwave; Sky; Optics; Detector","score_opus":0.013873810333133115,"score_gpt":0.23510366453963963,"score_spread":0.2212298542065065,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952332536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93532497,0.0009237604,0.016143618,0.0002235867,0.00006993204,0.00012717904,0.015102923,0.0025639327,0.02952016],"genre_scores_gemma":[0.9631472,0.0003957589,0.020728601,0.000092359616,0.00016051662,0.00009947579,0.012700461,0.0002964128,0.002379173],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99976677,0.000030222325,0.0000065049194,0.00006055719,0.00008578215,0.000050152277],"domain_scores_gemma":[0.99954385,0.000059641323,0.00016269236,0.000084484454,0.00006077642,0.000088527806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030301992,0.0004586962,0.0002763167,0.0015501175,0.00032908586,0.00044229077,0.00043464213,0.00035945248,0.0028696845],"category_scores_gemma":[0.0005349995,0.00026250147,0.00024407778,0.0011212517,0.00024192841,0.0004303511,0.0004469657,0.0005212583,0.00085054495],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022814553,0.0004233286,0.39660767,0.00058880425,0.00075140083,0.00079212704,0.0004728214,0.0033109188,0.4623225,0.00445251,0.018997172,0.10899922],"study_design_scores_gemma":[0.000103693594,0.000298076,0.8829458,0.000028370643,0.00012889096,0.0009278259,0.000065632594,0.004274258,0.08849332,0.0008271382,0.02186449,0.000042521562],"about_ca_topic_score_codex":0.000850114,"about_ca_topic_score_gemma":0.0024463185,"teacher_disagreement_score":0.0028696845,"about_ca_system_score_codex":0.00027595263,"about_ca_system_score_gemma":0.00014889298,"threshold_uncertainty_score":0.009600103},"labels":[],"label_agreement":null},{"id":"W2952339388","doi":"10.1088/0004-637x/726/2/66","title":"MASS TRANSFER IN BINARY STARS USING SMOOTHED PARTICLE HYDRODYNAMICS. I. NUMERICAL METHOD","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Smoothed-particle hydrodynamics; Binary number; Stars; Binary star; Boundary (topology); Mass transfer; Boundary value problem; RADIUS; Stellar mass","score_opus":0.014519461468965184,"score_gpt":0.30099878349683656,"score_spread":0.2864793220278714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952339388","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07611782,0.0006205121,0.90960395,0.0003418636,0.0001788345,0.00022273409,0.0002947715,0.0011728517,0.011446598],"genre_scores_gemma":[0.6899217,0.0005322212,0.29843837,0.00025155855,0.000136252,0.0006417533,0.00037839083,0.00047984772,0.009219928],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999796,0.00007977888,0.000011395915,0.000020819367,0.00006837393,0.000023578794],"domain_scores_gemma":[0.99905676,0.0003918282,0.00014311915,0.000117854666,0.00018750112,0.00010291297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071553345,0.00057848473,0.00094938575,0.0007608986,0.00075946137,0.0010529276,0.0016916244,0.0017396947,0.002478334],"category_scores_gemma":[0.002334976,0.00044607525,0.0008004263,0.0007368304,0.0011564482,0.00091292895,0.0010644109,0.00079681084,0.00058966555],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039722494,0.000048310867,0.0010754084,0.000053570904,0.000028042325,0.000080664024,0.000050207476,0.9680719,0.002277463,0.02144207,0.0005184559,0.006314261],"study_design_scores_gemma":[0.000009216876,0.0000053171,0.00006853873,0.000002365559,0.0000016498508,0.000006702427,0.0000028635884,0.99758005,0.00014821204,0.0018311645,0.0003400474,0.000003815226],"about_ca_topic_score_codex":0.009178668,"about_ca_topic_score_gemma":0.0041020755,"teacher_disagreement_score":0.009178668,"about_ca_system_score_codex":0.0013326767,"about_ca_system_score_gemma":0.0015398463,"threshold_uncertainty_score":0.018250465},"labels":[],"label_agreement":null},{"id":"W2952386684","doi":"10.3847/1538-4357/aae47a","title":"High-energy and Very High Energy Emission from Stellar-mass Black Holes Moving in Gaseous Clouds","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Black hole (networking); Astrophysics; Gamma ray; Event horizon; Magnetosphere; Intermediate-mass black hole; Electron; Accretion (finance); Spin-flip; Event (particle physics); Nuclear physics; Plasma","score_opus":0.005554154795672201,"score_gpt":0.19512700525031404,"score_spread":0.18957285045464184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952386684","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99799997,0.00013677134,0.0006341062,0.000026201711,0.0000038442413,0.0000051494935,0.000032098906,0.000016961341,0.0011448062],"genre_scores_gemma":[0.99952996,0.000035841214,0.00023043169,0.000008060924,0.000007221591,0.000001827277,0.000034346845,0.000004958979,0.00014738883],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999367,0.0000090398735,0.0000014400608,0.000011609753,0.000010771613,0.000030515657],"domain_scores_gemma":[0.99984753,0.00004991012,0.000038986764,0.000010562884,0.000012822674,0.000040167713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018203756,0.00033198463,0.0002641736,0.000567007,0.0004133817,0.00049613905,0.00040121205,0.00039095926,0.0009972573],"category_scores_gemma":[0.00020594397,0.00014683312,0.0003020502,0.00040907363,0.00043242594,0.0002259599,0.0005393753,0.00027913958,0.0001512437],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001537022,0.00038978676,0.23105101,0.00019653905,0.00031330227,0.006770176,0.0010783111,0.018856112,0.71159214,0.010890478,0.0010572837,0.016267896],"study_design_scores_gemma":[0.00023250381,0.0008148687,0.82308763,0.00005713334,0.0001646518,0.0022063304,0.0010062914,0.06495705,0.099646546,0.0054112864,0.0023539115,0.00006180381],"about_ca_topic_score_codex":0.0008713188,"about_ca_topic_score_gemma":0.0006312552,"teacher_disagreement_score":0.0009972573,"about_ca_system_score_codex":0.0002479453,"about_ca_system_score_gemma":0.00006191272,"threshold_uncertainty_score":0.0033361316},"labels":[],"label_agreement":null},{"id":"W2952544180","doi":"10.3847/1538-4357/ab203f","title":"The Effect of Minor and Major Mergers on the Evolution of Low-excitation Radio Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Fermilab; University of Hull; Max-Planck-Gesellschaft; Universität Basel; Drexel University; Alfred P. Sloan Foundation; Natural Sciences and Engineering Research Council of Canada; Johns Hopkins University; National Aeronautics and Space Administration; U.S. Department of Energy; Science and Technology Facilities Council; Case Western Reserve University; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Galaxy merger; Active galactic nucleus; Accretion (finance); Stellar mass; Galaxy; Population; Galaxy formation and evolution; Star formation; Medicine","score_opus":0.0028265956779448998,"score_gpt":0.18865849771097798,"score_spread":0.18583190203303307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952544180","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99975973,0.000038956656,0.000030364452,0.0000053834697,2.4157126e-7,5.589502e-7,0.000042824133,0.0000029561302,0.00011891974],"genre_scores_gemma":[0.9998222,0.000011615057,0.000027265243,0.0000036743968,0.0000010560909,4.1015906e-7,0.00008893881,9.654401e-7,0.00004386521],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997458,0.000049461127,0.000017441569,0.00008460724,0.00004702339,0.00005566216],"domain_scores_gemma":[0.99804175,0.00038462816,0.00083212537,0.00016365842,0.00013466977,0.00044315605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047712153,0.00020016552,0.00020389693,0.0011477848,0.00022426728,0.00075032725,0.0002668239,0.00020218262,0.0008358657],"category_scores_gemma":[0.0013040358,0.00013484173,0.00017816883,0.00040064525,0.00044747262,0.0003220672,0.00050497067,0.0001546598,0.00016178304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000087337765,0.000009907436,0.9924843,0.00000432516,0.000020784895,0.000036057732,0.00007510155,0.000075398864,0.0056891995,0.000031969885,0.000017980814,0.0014676632],"study_design_scores_gemma":[6.822153e-7,0.000019711704,0.9995608,6.1417677e-7,0.000004378079,0.00003439793,0.0000434882,0.000069665475,0.00023388426,0.00000745789,0.000024024252,8.432248e-7],"about_ca_topic_score_codex":0.0022692645,"about_ca_topic_score_gemma":0.003943247,"teacher_disagreement_score":0.0022692645,"about_ca_system_score_codex":0.00023876743,"about_ca_system_score_gemma":0.000082489605,"threshold_uncertainty_score":0.004512131},"labels":[],"label_agreement":null},{"id":"W2952571866","doi":"10.1088/0004-637x/791/2/88","title":"THE DEPENDENCE OF C IV BROAD ABSORPTION LINE PROPERTIES ON ACCOMPANYING Si IV AND Al III ABSORPTION: RELATING QUASAR-WIND IONIZATION LEVELS, KINEMATICS, AND COLUMN DENSITIES","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Ionization; Line (geometry); Equivalent width; Absorption (acoustics); Analytical Chemistry (journal); Absorption spectroscopy; Thermal ionization","score_opus":0.025950067183896315,"score_gpt":0.2372536342557065,"score_spread":0.2113035670718102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952571866","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998755,0.000039105234,0.00044119987,0.0000044469584,6.807434e-7,0.0000025809159,0.00018386912,0.000008921325,0.00056428893],"genre_scores_gemma":[0.99954706,0.000015695017,0.00016037263,0.000002219646,0.0000013843797,0.0000015723024,0.0001940866,0.000002673291,0.00007487145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999076,0.0000120443165,0.0000064408237,0.000033556615,0.000018721134,0.000021597289],"domain_scores_gemma":[0.998684,0.00042520367,0.00048322193,0.0001267565,0.00012994523,0.00015091515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025346092,0.00019851781,0.00012533537,0.00087758445,0.0001739487,0.00046393237,0.0002624757,0.00025413168,0.00064720516],"category_scores_gemma":[0.0011559635,0.00012476527,0.00018857168,0.00048228577,0.00023467085,0.0004659176,0.00028686502,0.00020175186,0.00020093919],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009766049,0.000036546553,0.9683594,0.0000096810945,0.000042582313,0.0000888574,0.00005046215,0.0019994823,0.026264427,0.000121799894,0.0000427088,0.0028863763],"study_design_scores_gemma":[0.0000011973855,0.00003791357,0.995246,9.986255e-7,0.0000065751215,0.00007505069,0.000028681125,0.002580451,0.0019025401,0.00005595183,0.00006151463,0.000003262423],"about_ca_topic_score_codex":0.0030830544,"about_ca_topic_score_gemma":0.0036868928,"teacher_disagreement_score":0.0030830544,"about_ca_system_score_codex":0.00020649926,"about_ca_system_score_gemma":0.00008050754,"threshold_uncertainty_score":0.0061302185},"labels":[],"label_agreement":null},{"id":"W2952616247","doi":"10.3847/1538-4357/ab2874","title":"A Massive Magnetic Helium Atmosphere White Dwarf Binary in a Young Star Cluster","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of British Columbia; University of British Columbia Hospital","funders":"","keywords":"White dwarf; Chandrasekhar limit; Star cluster; Open cluster; Stellar evolution; Binary star; Stellar classification; Cluster (spacecraft); Stellar mass","score_opus":0.005161836289140232,"score_gpt":0.20142571410777266,"score_spread":0.19626387781863242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952616247","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99955016,0.00001951108,0.000050144474,0.000010559038,0.0000016852829,0.0000026283424,0.00007617639,0.000005642529,0.00028348886],"genre_scores_gemma":[0.99905664,0.00001879916,0.0001629302,0.000016994449,0.0000049241917,0.000001880297,0.00025724425,0.000002675016,0.00047792355],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992955,0.0000050135213,0.000005030222,0.000022704176,0.000016258702,0.000021562057],"domain_scores_gemma":[0.9997718,0.000026492724,0.0000466835,0.00002144906,0.000024872093,0.000108608554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014351841,0.00015576581,0.0002282271,0.00064772135,0.0007185404,0.00039650602,0.00015659814,0.00017569096,0.0009086178],"category_scores_gemma":[0.00026375332,0.00006617686,0.00008517333,0.00045193033,0.00018886461,0.00016157815,0.00036857207,0.000134733,0.00033089228],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000117684816,0.00007427386,0.98113453,0.000014038849,0.000016475335,0.0035380477,0.00063898787,0.00017875276,0.010065166,0.0002737165,0.00035979127,0.0035886283],"study_design_scores_gemma":[0.0000060374946,0.0001773961,0.99321353,0.000003625571,0.000015248177,0.0019448221,0.00053986197,0.00041960372,0.0018429062,0.000094502946,0.0017358784,0.000006562971],"about_ca_topic_score_codex":0.005739905,"about_ca_topic_score_gemma":0.009442585,"teacher_disagreement_score":0.005739905,"about_ca_system_score_codex":0.0002241948,"about_ca_system_score_gemma":0.00019118669,"threshold_uncertainty_score":0.011412978},"labels":[],"label_agreement":null},{"id":"W2952663570","doi":"10.1088/0004-637x/801/1/15","title":"CONGLOMERATION OF KILOMETER-SIZED PLANETESIMALS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planetesimal; Planet; Asteroid; Cosmic dust; Infrared astronomy","score_opus":0.01997523695790345,"score_gpt":0.23478843966577662,"score_spread":0.21481320270787316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2952663570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99394083,0.0000797366,0.0052021653,0.000018343562,0.0000018906467,0.000004798988,0.000025767571,0.000032887398,0.00069364853],"genre_scores_gemma":[0.99635077,0.000046825196,0.0031173243,0.0000061426385,0.0000015629728,0.000007368207,0.000049590453,0.000010730191,0.0004097126],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998927,0.000023870056,0.0000061511037,0.00003893929,0.000017381826,0.00002092184],"domain_scores_gemma":[0.99847513,0.0008289343,0.0003294991,0.0001689352,0.00008651041,0.00011103136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026491136,0.00018199834,0.00016323605,0.0004236658,0.00030344172,0.0005238431,0.00058704143,0.00026494925,0.0008487206],"category_scores_gemma":[0.0032367753,0.00011959698,0.00019218792,0.00041668193,0.0005313729,0.000733447,0.0005264402,0.00024924392,0.00013505174],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003820882,0.00015079814,0.3726093,0.00011667387,0.00016051091,0.0011651126,0.0008998374,0.5237793,0.04512796,0.024503982,0.0005579124,0.030546578],"study_design_scores_gemma":[0.000018019065,0.00014357376,0.054802347,0.000007617182,0.00003749312,0.00051004137,0.0002667052,0.92251605,0.01713556,0.003327101,0.0012140863,0.000021512877],"about_ca_topic_score_codex":0.0018280352,"about_ca_topic_score_gemma":0.0015106946,"teacher_disagreement_score":0.0018280352,"about_ca_system_score_codex":0.0003397572,"about_ca_system_score_gemma":0.00012259145,"threshold_uncertainty_score":0.0036347508},"labels":[],"label_agreement":null},{"id":"W2953064028","doi":"10.1088/0004-637x/809/1/81","title":"<i>HERSCHEL</i>OBSERVATIONS OF THE W3 GMC (II): CLUES TO THE FORMATION OF CLUSTERS OF HIGH-MASS STARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of Victoria; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Star formation; Stars; Initial mass function; Star cluster; Mass segregation; Stellar mass; Stellar evolution; Log-normal distribution; Astronomy; Statistics","score_opus":0.024741948803566147,"score_gpt":0.24157439005724082,"score_spread":0.21683244125367468,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953064028","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9802146,0.00025051835,0.0019225648,0.00027295828,0.000013814915,0.00003142544,0.005954411,0.0003438798,0.01099574],"genre_scores_gemma":[0.9864581,0.000088544584,0.0051698703,0.00015528874,0.000028138618,0.000022396374,0.005135404,0.0001050678,0.00283723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995184,0.0000026523624,0.0000017008305,0.000008940709,0.000017719038,0.000017161226],"domain_scores_gemma":[0.9998274,0.000011550783,0.000052236708,0.000031227144,0.00003224379,0.00004528538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015558886,0.000149161,0.00008934362,0.00083222974,0.00039382948,0.0003935923,0.0002181736,0.00026645706,0.0021507947],"category_scores_gemma":[0.0001607431,0.000066312925,0.00019117155,0.00089858385,0.00019136068,0.00030207584,0.0005032828,0.00029263063,0.0006701755],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003830123,0.00010430848,0.77145207,0.0001154147,0.00011635142,0.0006562681,0.0008656252,0.0014246405,0.15394124,0.0017311141,0.013484921,0.055725005],"study_design_scores_gemma":[0.000008599475,0.00002743437,0.9827307,0.000008184497,0.0000102559625,0.00014082952,0.00014348188,0.00083473115,0.006096922,0.0002142834,0.009776998,0.0000075232765],"about_ca_topic_score_codex":0.023711896,"about_ca_topic_score_gemma":0.058757618,"teacher_disagreement_score":0.023711896,"about_ca_system_score_codex":0.00046685606,"about_ca_system_score_gemma":0.0001807823,"threshold_uncertainty_score":0.04714775},"labels":[],"label_agreement":null},{"id":"W2953159743","doi":"10.3847/1538-4357/ab2c6e","title":"A Search of TESS Full-frame Images for a Simultaneous Optical Counterpart to FRB 181228","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Fast radio burst; Exoplanet; Limiting magnitude; Millisecond; Radio telescope; Flux (metallurgy); Population; Galaxy; Astrometry; Telescope","score_opus":0.008958149822430438,"score_gpt":0.2588712207159516,"score_spread":0.24991307089352116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953159743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99233866,0.00017704371,0.0008921121,0.0001986026,0.000026301599,0.000017980694,0.0018517314,0.00019622555,0.004301354],"genre_scores_gemma":[0.9946971,0.00002723565,0.0016382812,0.00005626972,0.000027109267,0.000008132998,0.0029641273,0.00002324227,0.00055838615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984396,0.0000078947305,0.00000778848,0.000045020097,0.000054366836,0.000041006824],"domain_scores_gemma":[0.9991353,0.00008262151,0.00027077144,0.00007727804,0.00016650037,0.00026763193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031017937,0.00019985944,0.0002549809,0.0016095272,0.000551946,0.00043078247,0.0003667694,0.00039862117,0.0036968973],"category_scores_gemma":[0.0005933964,0.00020243014,0.00032328357,0.0006873515,0.00019814,0.0002522639,0.00042127722,0.00024507,0.00076254964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010070208,0.00021791506,0.6360831,0.00015781749,0.00019072529,0.0025567103,0.00048448434,0.0011341748,0.30373526,0.001048797,0.008642853,0.044741254],"study_design_scores_gemma":[0.000033902033,0.00015749809,0.97702754,0.000024373538,0.00004331106,0.00087468105,0.00022475475,0.0041467845,0.01143458,0.00013990786,0.005876636,0.000016020358],"about_ca_topic_score_codex":0.00420057,"about_ca_topic_score_gemma":0.010460519,"teacher_disagreement_score":0.00420057,"about_ca_system_score_codex":0.00052692695,"about_ca_system_score_gemma":0.00024723617,"threshold_uncertainty_score":0.012367308},"labels":[],"label_agreement":null},{"id":"W2953218312","doi":"10.3847/1538-4357/ab27cb","title":"CHANG-ES. XVII. Hα Imaging of Nearby Edge-on Galaxies, New SFRs, and an Extreme Star Formation Region—Data Release 2","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Calgary","funders":"","keywords":"Star formation; Galaxy; Stars; Extinction (optical mineralogy); Halo; Accretion (finance); Star (game theory); Scale (ratio)","score_opus":0.02119180226297045,"score_gpt":0.2278043665375325,"score_spread":0.20661256427456204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953218312","genre_codex":"empirical","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92973024,0.00020290192,0.00084656925,0.00006147561,0.000025333939,0.00008936762,0.062635094,0.00047642982,0.005932622],"genre_scores_gemma":[0.75438696,0.00013434092,0.0047188518,0.00013776906,0.000034252153,0.00015199989,0.23442212,0.00018978093,0.005823979],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999796,0.000014413949,0.000018500043,0.000051408417,0.0000734182,0.000046382153],"domain_scores_gemma":[0.99875104,0.00008604074,0.00021887451,0.00023807026,0.0003939309,0.0003119961],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060487824,0.00039319904,0.00028246868,0.0019641118,0.00035019527,0.000615708,0.00042589556,0.00029085245,0.0034530705],"category_scores_gemma":[0.0005496109,0.0002971525,0.00030886146,0.0014162922,0.00012181582,0.00035973405,0.0006025169,0.00019974246,0.001595584],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031307514,0.00008595497,0.9519305,0.00007361969,0.000093203096,0.00021502262,0.00018079579,0.00035914444,0.018670853,0.00006504875,0.008600696,0.019412024],"study_design_scores_gemma":[0.000014132104,0.000024191584,0.9903324,0.0000070823216,0.000015976766,0.00009451042,0.00005512565,0.0002606601,0.0026155545,0.000012703941,0.006560987,0.000006569833],"about_ca_topic_score_codex":0.016959915,"about_ca_topic_score_gemma":0.056182113,"teacher_disagreement_score":0.016959915,"about_ca_system_score_codex":0.00040919887,"about_ca_system_score_gemma":0.00028523823,"threshold_uncertainty_score":0.0337224},"labels":[],"label_agreement":null},{"id":"W2953236618","doi":"10.3847/0004-637x/823/1/65","title":"THE FIRST COMBINED SEARCH FOR NEUTRINO POINT-SOURCES IN THE SOUTHERN HEMISPHERE WITH THE ANTARES AND ICECUBE NEUTRINO TELESCOPES","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Alberta","funders":"Office of Polar Programs; Japan Society for the Promotion of Science; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Helmholtz Alliance for Astroparticle Physics; Conseil Régional d'Alsace; Istituto Nazionale di Fisica Nucleare; Conseil Régional Provence-Alpes-Côte d'Azur; Agence de l'Oriental; Centre National pour la Recherche Scientifique et Technique; Centre National de la Recherche Scientifique; Knut och Alice Wallenbergs Stiftelse; National Research Foundation of Korea; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Generalitat Valenciana; Ministerio de Economía y Competitividad; Polarforskningssekretariatet; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Stichting voor Fundamenteel Onderzoek der Materie; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; National Research Foundation; Autoritatea Natională pentru Cercetare Stiintifică; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; European Commission; Western Canada Research Grid; Vlaamse regering; University of Oxford; Compute Canada; Conseil Régional, Île-de-France; Fonds De La Recherche Scientifique - FNRS; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Neutrino; Sky; Astrophysics; Neutrino detector; Astronomy; Point source; Astroparticle physics; Flux (metallurgy); Southern Hemisphere; Neutrino astronomy; Neutrino oscillation; Particle physics","score_opus":0.0068612444487495435,"score_gpt":0.20757568543020335,"score_spread":0.2007144409814538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953236618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9765326,0.0016665731,0.0069287806,0.00020293104,0.000046995006,0.00014531653,0.005921887,0.00032566633,0.00822922],"genre_scores_gemma":[0.96063733,0.0006549365,0.025646128,0.00010877776,0.00011338368,0.00011934406,0.010983247,0.00011113805,0.0016257353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99872726,0.0002681356,0.000037507703,0.00024637865,0.0005716573,0.00014903798],"domain_scores_gemma":[0.9979182,0.00055060594,0.00043898134,0.0002476614,0.000549497,0.00029507698],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015590859,0.0006646607,0.001016142,0.002059163,0.00050452614,0.0010250161,0.00040428873,0.00048154002,0.001495921],"category_scores_gemma":[0.0012897815,0.00045047744,0.0009809247,0.0019136883,0.0002979099,0.0006145706,0.0013140116,0.00043820366,0.00042986995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0033122816,0.00024678602,0.7461037,0.00031051858,0.0020184305,0.0010750666,0.00042471217,0.004620282,0.14150304,0.0007851727,0.0051792744,0.09442079],"study_design_scores_gemma":[0.00013330633,0.00041823805,0.9595554,0.000050400882,0.0005009706,0.00080764166,0.00018285238,0.004666335,0.020885965,0.00043404088,0.012306642,0.000058170554],"about_ca_topic_score_codex":0.0062175165,"about_ca_topic_score_gemma":0.018697212,"teacher_disagreement_score":0.0062175165,"about_ca_system_score_codex":0.0004666961,"about_ca_system_score_gemma":0.0006898965,"threshold_uncertainty_score":0.012362659},"labels":[],"label_agreement":null},{"id":"W2953256143","doi":"10.1086/421344","title":"Erratum: “Evidence for Planet‐induced Chromospheric Activity on HD 179949” (ApJ, 597, 1092 [2003])","year":2004,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Planet; Astrobiology; Physics; Astronomy","score_opus":0.02559540787698075,"score_gpt":0.2769030446711986,"score_spread":0.25130763679421786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953256143","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.002915321,0.0021864197,0.00082422636,0.052284714,0.9214096,0.00007497881,0.0031163418,0.0006671543,0.016521255],"genre_scores_gemma":[0.054952502,0.014113208,0.0083432915,0.12268444,0.1684735,0.00024202059,0.0161489,0.0018240862,0.613218],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99917287,0.00008007076,0.00020784527,0.00013035694,0.00032487378,0.000084015286],"domain_scores_gemma":[0.9937202,0.0009708741,0.00056207913,0.00048538286,0.0038152116,0.00044620637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010314077,0.0020643577,0.0009258219,0.0031219176,0.0034607584,0.0016908251,0.0021283296,0.0034425997,0.029713934],"category_scores_gemma":[0.011291528,0.0008250008,0.0009244309,0.0017168778,0.0010858662,0.0014884108,0.0010472185,0.0036160115,0.021705074],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005851837,0.000026632752,0.00056030334,0.00012489824,0.000016137688,0.0008143197,0.00004318542,0.000053234955,0.0002788187,0.00025079245,0.98963076,0.008142487],"study_design_scores_gemma":[0.000044314806,0.00006642425,0.012605233,0.00027372123,0.00006480433,0.0010778938,0.00019210871,0.00024537172,0.0009967652,0.0005361261,0.98384064,0.00005659125],"about_ca_topic_score_codex":0.03715598,"about_ca_topic_score_gemma":0.045764063,"teacher_disagreement_score":0.03715598,"about_ca_system_score_codex":0.0024493516,"about_ca_system_score_gemma":0.0020240133,"threshold_uncertainty_score":0.09940302},"labels":[],"label_agreement":null},{"id":"W2953275124","doi":"10.3847/1538-4357/ab2be6","title":"KSP-SN-2016kf: A Long-rising H-rich Type II Supernova with Unusually High <sup>56</sup>Ni Mass Discovered in the KMTNet Supernova Program","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Supernova; Light curve; Red supergiant; Metallicity; Type II supernova; RADIUS; Galaxy; Luminosity; Supergiant","score_opus":0.008762124416661363,"score_gpt":0.23175518140024837,"score_spread":0.222993056983587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953275124","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99776924,0.000052026422,0.0003653849,0.000023809824,0.000016609956,0.000013807759,0.0005435773,0.000065001215,0.0011505332],"genre_scores_gemma":[0.997488,0.00003914199,0.00043368083,0.000015255306,0.000008381082,0.0000054768516,0.0013102292,0.00001685603,0.0006830668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992883,0.000004365397,0.0000066028847,0.00001797572,0.000020259295,0.000022010936],"domain_scores_gemma":[0.99971575,0.000019940058,0.00006191158,0.000033731183,0.00002559058,0.00014304936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021085028,0.00037544343,0.00028640154,0.0004740251,0.00042168703,0.00045779246,0.00031369212,0.00022750904,0.0010396191],"category_scores_gemma":[0.00029712982,0.0001095182,0.00037101936,0.00029269257,0.0002943411,0.0002112169,0.00054219813,0.00030698968,0.0003209567],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008360959,0.00017406093,0.92213625,0.00008285942,0.00019254959,0.012296426,0.00017907553,0.0040966044,0.040838514,0.001536867,0.0013845781,0.01624608],"study_design_scores_gemma":[0.00003889001,0.0002992311,0.96023047,0.000020752657,0.000057741734,0.010583683,0.00019601572,0.0078189485,0.0152413845,0.0006634833,0.0048259753,0.00002346886],"about_ca_topic_score_codex":0.0033241527,"about_ca_topic_score_gemma":0.0055962875,"teacher_disagreement_score":0.0033241527,"about_ca_system_score_codex":0.00038693205,"about_ca_system_score_gemma":0.00021309733,"threshold_uncertainty_score":0.0066096187},"labels":[],"label_agreement":null},{"id":"W2953418954","doi":"10.3847/1538-4357/ab212a","title":"The z = 0.54 LoBAL Quasar SDSS J085053.12+445122.5. II. The Nature of Partial Covering in the Broad-absorption-line Outflow","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; Western University","funders":"Space Telescope Science Institute","keywords":"Physics; Quasar; Astrophysics; Outflow; Infrared; Spectral line; Extrapolation; Absorption (acoustics); Emission spectrum; Absorption spectroscopy; Rest frame; Optical depth; Redshift; Astronomy; Galaxy; Optics","score_opus":0.006210066327040444,"score_gpt":0.22192796105750331,"score_spread":0.21571789473046288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2953418954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99640083,0.00008114528,0.0003198462,0.000038881495,0.000004638112,0.0000035492656,0.0010595983,0.000059988182,0.002031667],"genre_scores_gemma":[0.9982135,0.000014900671,0.00015826875,0.000015652864,0.0000048626653,0.0000017655262,0.0013008241,0.0000062703393,0.00028389142],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993455,0.000009137433,0.0000030241165,0.00001779891,0.000013388762,0.000022150254],"domain_scores_gemma":[0.999703,0.00004856566,0.000090815534,0.000041205192,0.0000421593,0.00007424627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023273299,0.00014459921,0.0001717349,0.00078586955,0.00022457071,0.00034559125,0.00016289104,0.00013785363,0.0016086869],"category_scores_gemma":[0.00037862797,0.00007901836,0.00012737601,0.00035835482,0.00013758037,0.00023794611,0.00024117163,0.00012497733,0.0003333627],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039597575,0.00012940673,0.92329687,0.000050210598,0.00011142693,0.00029842948,0.00019334652,0.0012974027,0.052229762,0.0012386765,0.0029376706,0.017820833],"study_design_scores_gemma":[0.000004600922,0.000017658745,0.996824,0.0000020972873,0.0000067003375,0.00003631154,0.00004623132,0.0018180235,0.00064892875,0.00009612663,0.00049636984,0.0000029765736],"about_ca_topic_score_codex":0.0050002863,"about_ca_topic_score_gemma":0.0068976944,"teacher_disagreement_score":0.0050002863,"about_ca_system_score_codex":0.00023984986,"about_ca_system_score_gemma":0.00004786703,"threshold_uncertainty_score":0.009942353},"labels":[],"label_agreement":null},{"id":"W2954075881","doi":"10.3847/1538-4357/ab7ea6","title":"An Examination of Galactic Polarization with Application to the Planck TB Correlation","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Polarization (electrochemistry); Astrophysics; Brewster's angle; Planck; Cosmic microwave background; Correlation; Microwave; Linear polarization; Computational physics; Optics; Geometry; Quantum mechanics; Chemistry","score_opus":0.007180549662921611,"score_gpt":0.2196984668693454,"score_spread":0.2125179172064238,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954075881","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939442,0.00004718571,0.0033486001,0.00004704503,0.000003114723,0.0000039758934,0.0005834028,0.00013749996,0.0018850316],"genre_scores_gemma":[0.99929297,0.000013127322,0.00048939016,0.0000037219158,0.0000021680405,0.0000015538592,0.00015364433,0.000012778851,0.00003066317],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999859,0.000046458703,0.000006104112,0.00003586645,0.00002580527,0.000026682474],"domain_scores_gemma":[0.99900824,0.00048185492,0.000200612,0.00016914716,0.00009258366,0.00004759989],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055390445,0.00018861357,0.00015451667,0.00086258556,0.00020490077,0.0005697295,0.00019818665,0.00018849527,0.0014560228],"category_scores_gemma":[0.0022347027,0.00013917401,0.0003208796,0.0016830004,0.0002594161,0.000284839,0.0002784156,0.00020905124,0.0001385773],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002485851,0.000051195602,0.6961614,0.00007454104,0.00032033192,0.00048714527,0.00033401116,0.24345325,0.021563588,0.0080112275,0.0020447457,0.027250007],"study_design_scores_gemma":[0.000011411186,0.000030978616,0.6776001,0.000009976924,0.0000422225,0.00015692471,0.00012546018,0.313418,0.0055028102,0.0018939523,0.0011782876,0.000029834975],"about_ca_topic_score_codex":0.007663561,"about_ca_topic_score_gemma":0.0026414946,"teacher_disagreement_score":0.007663561,"about_ca_system_score_codex":0.0003640535,"about_ca_system_score_gemma":0.0001591081,"threshold_uncertainty_score":0.015237868},"labels":[],"label_agreement":null},{"id":"W2954251221","doi":"10.3847/1538-4357/ab2d9c","title":"The Molecular Outflow in NGC 253 at a Resolution of Two Parsecs","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Outflow; Luminosity; Kinetic energy; Bipolar outflow; Protostar; Star formation; Submillimeter Array","score_opus":0.006843605625901112,"score_gpt":0.23575211960201536,"score_spread":0.22890851397611425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954251221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961867,0.00020855461,0.0015783274,0.000036449463,0.000007581764,0.0000067016504,0.00054888654,0.0002666864,0.0011601415],"genre_scores_gemma":[0.99699116,0.000055972225,0.0020528114,0.000018038656,0.000007426342,0.000005604639,0.0006912877,0.000015054753,0.00016257257],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988985,0.000009256657,0.000008167546,0.00004348804,0.000025594938,0.000023499246],"domain_scores_gemma":[0.99971515,0.000060146576,0.00006898411,0.000038339458,0.000060414357,0.00005695465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030662783,0.00021710018,0.0002485837,0.0003751699,0.0002867849,0.00062566204,0.00034227697,0.0002665099,0.000890662],"category_scores_gemma":[0.0005767387,0.0001957152,0.0002906811,0.00030131705,0.00015441696,0.00019810181,0.00025366544,0.00021627912,0.00025385054],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008606085,0.00025834094,0.67806023,0.00016626304,0.000430791,0.0027776095,0.00068573566,0.031802665,0.2361589,0.0015361486,0.0024554327,0.044807293],"study_design_scores_gemma":[0.000056505614,0.000079245154,0.94915265,0.000026926784,0.00013248014,0.00043399972,0.00020635295,0.034367844,0.01204218,0.0003679711,0.0031025454,0.000031277403],"about_ca_topic_score_codex":0.0167468,"about_ca_topic_score_gemma":0.019415794,"teacher_disagreement_score":0.0167468,"about_ca_system_score_codex":0.00074180134,"about_ca_system_score_gemma":0.00032506094,"threshold_uncertainty_score":0.03329861},"labels":[],"label_agreement":null},{"id":"W2954744376","doi":"10.3847/1538-4357/ab2da0","title":"Measurements of the Cross-spectra of the Cosmic Infrared and Microwave Backgrounds from 95 to 1200 GHz","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"High Energy Physics; National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Science; Centre National de la Recherche Scientifique; UK Space Agency; McGill University; University of Chicago; Canada Research Chairs; National Science Foundation; Imperial College London; National Aeronautics and Space Administration; Argonne National Laboratory; U.S. Department of Energy; California Institute of Technology; Centre National d’Etudes Spatiales; Gordon and Betty Moore Foundation","keywords":"Cosmic infrared background; Cosmic microwave background; Spectral line; Multipole expansion; Microwave; Planck; Cosmic background radiation; Spectral density; Infrared","score_opus":0.012107166606816176,"score_gpt":0.22164674008293564,"score_spread":0.20953957347611946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954744376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952042,0.00016635249,0.0016295939,0.000016195117,0.000006149858,0.000002919936,0.00057072775,0.00010432135,0.002299479],"genre_scores_gemma":[0.99794966,0.00006959572,0.0005341406,0.000008611657,0.000009217758,0.0000037457007,0.0011797498,0.000022643215,0.00022265913],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985313,0.00001568662,0.0000054569214,0.000049531816,0.00005001165,0.000026067504],"domain_scores_gemma":[0.99968207,0.00006456623,0.000089892594,0.000039754552,0.00006140352,0.00006238524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021664504,0.00025770845,0.00012708253,0.001330972,0.00013572602,0.00029699985,0.00016491755,0.00015700287,0.0013739177],"category_scores_gemma":[0.00066846784,0.00014114489,0.000121726305,0.0010868546,0.00012383424,0.00019951329,0.00030854892,0.00024476944,0.0003644568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086998387,0.00015725737,0.7365236,0.00011619962,0.00029861435,0.00022476293,0.0005061393,0.0033164932,0.16868146,0.0012329032,0.0018227653,0.08624977],"study_design_scores_gemma":[0.0000051937523,0.000028472787,0.9908228,0.000004279955,0.00002115393,0.00011950245,0.000021079439,0.0009746258,0.006512413,0.00007849085,0.0014064028,0.0000056815106],"about_ca_topic_score_codex":0.0011899995,"about_ca_topic_score_gemma":0.0012150655,"teacher_disagreement_score":0.0013739177,"about_ca_system_score_codex":0.00014127967,"about_ca_system_score_gemma":0.000036294074,"threshold_uncertainty_score":0.0045962334},"labels":[],"label_agreement":null},{"id":"W2954805577","doi":"10.3847/1538-4357/ab4354","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Accretion and Broad Emission Line Physics from a Hypervariable Quasar","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Quasar; Reverberation mapping; Sky; Astronomy; Accretion (finance); Emission spectrum; Gravitational microlensing; Luminosity; Active galactic nucleus; Spectral line; Stars; Galaxy","score_opus":0.021404452335586004,"score_gpt":0.23876145916694572,"score_spread":0.21735700683135972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954805577","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960167,0.00007811429,0.00023042814,0.00004659393,0.0000032350217,0.0000063568846,0.0030449429,0.00004254094,0.0005311103],"genre_scores_gemma":[0.9818912,0.00006886956,0.0009596436,0.000024368373,0.000015108001,0.000008888713,0.016624345,0.000022035723,0.00038539732],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997267,0.00004691007,0.000013311533,0.000048389647,0.000089750974,0.000074905765],"domain_scores_gemma":[0.9989974,0.0001178896,0.00037498013,0.0001597849,0.00013088486,0.00021909684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067043386,0.00028066256,0.00017813826,0.0022250323,0.00030017848,0.00060779025,0.00028988294,0.00017578028,0.00067413814],"category_scores_gemma":[0.0006665505,0.00010382966,0.00028475077,0.0017283346,0.00022223723,0.00025977744,0.00063532504,0.00019502688,0.0002552514],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014665959,0.0001557538,0.9718981,0.000036108784,0.00017250952,0.00047004072,0.00028110246,0.002677148,0.0051687895,0.0003316195,0.0040211175,0.014641063],"study_design_scores_gemma":[0.0000044942194,0.00001382089,0.9964091,0.0000024313426,0.00001205484,0.000072157076,0.000078467376,0.0014071538,0.00045974087,0.00005179047,0.001484502,0.00000413437],"about_ca_topic_score_codex":0.018234266,"about_ca_topic_score_gemma":0.025822258,"teacher_disagreement_score":0.018234266,"about_ca_system_score_codex":0.00032004065,"about_ca_system_score_gemma":0.00029597207,"threshold_uncertainty_score":0.036256254},"labels":[],"label_agreement":null},{"id":"W2954884359","doi":"10.3847/1538-4357/ab2e03","title":"Northern Galactic Molecular Cloud Clumps in Hi-GAL: Clump and Star Formation within Clouds","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Star formation; Galactic plane; Molecular cloud; Milky Way; Line (geometry); Infrared; Galaxy; Virial mass; Galactic Center","score_opus":0.006141394075212805,"score_gpt":0.2176636594342362,"score_spread":0.2115222653590234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2954884359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99974054,0.000043968463,0.00004805107,0.0000076140377,4.7831884e-7,9.230835e-7,0.000043165724,0.0000021621922,0.00011311593],"genre_scores_gemma":[0.99988794,0.000009028482,0.000018552719,0.0000027677406,0.0000011519309,4.292052e-7,0.000051840852,9.613111e-7,0.000027174829],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997851,0.00003865764,0.000014744381,0.00004947218,0.000044866876,0.00006722539],"domain_scores_gemma":[0.9963983,0.0011175653,0.0014697736,0.000195443,0.00023777394,0.0005810365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005555308,0.00014192968,0.00028486698,0.0011569093,0.00031046927,0.00088659563,0.00043608368,0.00043941592,0.0013189424],"category_scores_gemma":[0.0025057576,0.00013220122,0.00020447903,0.0010734408,0.00044931954,0.00039086572,0.0005933656,0.00022173623,0.00023209942],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004218782,0.000011748229,0.997624,0.0000044771114,0.000019998748,0.00005523211,0.00005577705,0.0003975745,0.0010684762,0.000049880404,0.000027156826,0.00064356474],"study_design_scores_gemma":[0.0000020768944,0.000017093742,0.99841714,0.0000020650618,0.0000059402846,0.000036403755,0.000084883526,0.0011501887,0.00020604215,0.000038294023,0.00003793255,0.0000018330785],"about_ca_topic_score_codex":0.007897594,"about_ca_topic_score_gemma":0.008286314,"teacher_disagreement_score":0.007897594,"about_ca_system_score_codex":0.00053934514,"about_ca_system_score_gemma":0.000133797,"threshold_uncertainty_score":0.01570326},"labels":[],"label_agreement":null},{"id":"W2955163406","doi":"10.3847/1538-4357/ab2d27","title":"Presolar Silicon Carbide Grains of Types Y and Z: Their Molybdenum Isotopic Compositions and Stellar Origins","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; TRIUMF","funders":"National Aeronautics and Space Administration","keywords":"Nucleosynthesis; Asymptotic giant branch; Presolar grains; Metallicity; Stellar nucleosynthesis; Isotope; s-process; Stars; Molybdenum","score_opus":0.004920599912255456,"score_gpt":0.19450825499420005,"score_spread":0.18958765508194458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955163406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99940276,0.000060976654,0.000060917773,0.0000014606628,6.274599e-7,0.0000013967534,0.00011248969,0.000002888606,0.00035647917],"genre_scores_gemma":[0.9995172,0.000023611683,0.00009773414,0.0000017985643,8.6281904e-7,0.0000010704175,0.00018058778,0.000002417836,0.00017469864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999954,0.000002459026,0.0000038029884,0.00001305865,0.000012547081,0.000014168598],"domain_scores_gemma":[0.9998919,0.0000146416005,0.000037529353,0.000009794002,0.000027916003,0.000018260298],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006757401,0.00016421801,0.00017890937,0.0008575259,0.00028892964,0.00046591336,0.00014148148,0.00014369492,0.0011454375],"category_scores_gemma":[0.00012344577,0.00008513418,0.000110149114,0.00043335816,0.00023379698,0.00013289055,0.00020395583,0.000079448284,0.00023393457],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011622274,0.000030455976,0.5718895,0.000041153955,0.00005457288,0.00045592414,0.00030852814,0.00023370732,0.4155806,0.00021959336,0.00008441859,0.009939328],"study_design_scores_gemma":[0.000010545704,0.0001199078,0.95661867,0.0000026761284,0.000018818046,0.000345555,0.00018095714,0.00052976154,0.041195948,0.00007357774,0.00090005586,0.000003458573],"about_ca_topic_score_codex":0.00217291,"about_ca_topic_score_gemma":0.0025793444,"teacher_disagreement_score":0.00217291,"about_ca_system_score_codex":0.00018821671,"about_ca_system_score_gemma":0.000066537476,"threshold_uncertainty_score":0.0043205023},"labels":[],"label_agreement":null},{"id":"W2955186154","doi":"10.3847/1538-4357/ab3eb5","title":"The Evolution of O i over 3.2 &lt; z &lt; 6.5: Reionization of the Circumgalactic Medium","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; Universidad de Chile","keywords":"Physics; Reionization; Intergalactic medium; Astrophysics; Astronomy; Galaxy; Redshift","score_opus":0.0038984297992193263,"score_gpt":0.19403851618604354,"score_spread":0.1901400863868242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955186154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999395,0.00005377907,0.00005404535,0.00001518376,9.1579216e-7,0.0000011116365,0.00020155915,0.000008767578,0.00026966602],"genre_scores_gemma":[0.99940467,0.000031393003,0.00007009855,0.000009293268,0.00000265127,9.2161775e-7,0.00032264585,0.00000383124,0.00015457776],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986327,0.0000109318025,0.000005498046,0.000034881865,0.0000385167,0.000046972527],"domain_scores_gemma":[0.9990915,0.000072951625,0.0004562991,0.0000415348,0.000091496244,0.0002462155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002315135,0.00023904192,0.00019456957,0.0012385891,0.0002459309,0.00066700135,0.00028135756,0.00031661344,0.00088747306],"category_scores_gemma":[0.0005577009,0.00013052263,0.00024546823,0.0006956666,0.0002459628,0.00038623993,0.0005241493,0.00028783348,0.0003002088],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000063303705,0.000022070511,0.98967546,0.0000069078837,0.000028669132,0.00009257784,0.00017241602,0.00018552855,0.007129819,0.00006077799,0.00013536484,0.0024271281],"study_design_scores_gemma":[4.4133424e-7,0.000008291057,0.9994524,6.935717e-7,0.0000026268374,0.00004381592,0.00003528133,0.00011439504,0.00021568431,0.0000080150585,0.000117212876,0.0000010986438],"about_ca_topic_score_codex":0.004776877,"about_ca_topic_score_gemma":0.005072689,"teacher_disagreement_score":0.004776877,"about_ca_system_score_codex":0.00031381744,"about_ca_system_score_gemma":0.000076119824,"threshold_uncertainty_score":0.009498119},"labels":[],"label_agreement":null},{"id":"W2955397079","doi":"10.3847/1538-4357/ab2d2d","title":"Compact Disks in a High-resolution ALMA Survey of Dust Structures in the Taurus Molecular Cloud","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":252,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Astrophysics; Physics; Stars; Millimeter; Submillimeter Array; Debris disk; Planet; Molecular cloud; Spectral resolution; Protoplanetary disk; Star formation; Astronomy; Spectral line; Planetary system","score_opus":0.013076142288710527,"score_gpt":0.2530792401509277,"score_spread":0.24000309786221719,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955397079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994779,0.00006888703,0.00008805861,0.000008550383,9.235251e-7,0.0000027915396,0.00017126785,0.00000909689,0.00017242158],"genre_scores_gemma":[0.9992481,0.00002868296,0.00025504525,0.0000072363673,0.000005834153,0.0000025401625,0.00035911446,0.0000020174025,0.0000913809],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998634,0.000017242106,0.000009148188,0.00004175402,0.000037162765,0.00003121252],"domain_scores_gemma":[0.9996697,0.0000328285,0.00010968975,0.000036760077,0.00005476253,0.00009627967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018503351,0.00016520308,0.00021527369,0.001329867,0.0003408499,0.00058185146,0.00021926971,0.00020441567,0.00056443474],"category_scores_gemma":[0.0003836464,0.00016698602,0.0001381098,0.00069875823,0.00012504612,0.00032144238,0.00045044848,0.00013355252,0.00020164224],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013042915,0.00005936742,0.96708184,0.000019540998,0.000064123386,0.0002447161,0.00040403794,0.00018015469,0.0250823,0.000040856637,0.00024172997,0.0064509194],"study_design_scores_gemma":[0.0000029750302,0.000023271215,0.9987312,0.0000020562888,0.000010049963,0.00011327665,0.0001268509,0.00038511632,0.0003321093,0.000009147385,0.0002625583,0.0000014498586],"about_ca_topic_score_codex":0.0051973625,"about_ca_topic_score_gemma":0.011232824,"teacher_disagreement_score":0.0051973625,"about_ca_system_score_codex":0.00022068,"about_ca_system_score_gemma":0.000093249466,"threshold_uncertainty_score":0.010334253},"labels":[],"label_agreement":null},{"id":"W2955428058","doi":"10.3847/1538-4357/ab2b3a","title":"The Rest-frame <i>H</i>-band Luminosity Function of Red-sequence Galaxies in Clusters at 1.0 &lt; <i>z</i> &lt; 1.3","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Waterloo; York University","funders":"Astrophysics Division; Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; California Institute of Technology; Ministerio de Ciencia, Tecnología e Innovación Productiva; Jet Propulsion Laboratory; Centro de Astrofísica y Tecnologías Afines; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Luminosity function; Galaxy; Luminosity; Redshift; Galaxy cluster; Cluster (spacecraft); Luminous infrared galaxy; Elliptical galaxy","score_opus":0.0075662187956294594,"score_gpt":0.20298452255747507,"score_spread":0.1954183037618456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955428058","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994203,0.00003695242,0.000039654446,0.000007372899,6.4406476e-7,0.0000010786754,0.00032036754,0.000011786129,0.00016187341],"genre_scores_gemma":[0.9988863,0.000016983646,0.00006822851,0.0000066254547,0.0000023839423,0.000002013169,0.00086664886,0.0000044403805,0.00014650883],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998528,0.000008103399,0.0000062855797,0.00005134955,0.000020486696,0.000060903836],"domain_scores_gemma":[0.99909997,0.00010144404,0.00031084448,0.00006475994,0.00012825943,0.0002947631],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030274558,0.00023397003,0.00025525526,0.0016520725,0.00045005657,0.0005259444,0.00037912623,0.00031303277,0.001514208],"category_scores_gemma":[0.00056571653,0.0001849275,0.00028357795,0.00071436935,0.0002807905,0.0003131904,0.00040472313,0.00027321273,0.00055644754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018278045,0.000029138133,0.9894509,0.000009943122,0.00003715008,0.0000458499,0.00030756506,0.0004387555,0.0064770686,0.00006718637,0.00035306625,0.0026006934],"study_design_scores_gemma":[8.3784863e-7,0.0000067344513,0.9996124,5.179696e-7,0.00000447344,0.000015184166,0.000031603395,0.00015438403,0.00013386128,0.000007001312,0.00003159917,0.0000014319779],"about_ca_topic_score_codex":0.020509413,"about_ca_topic_score_gemma":0.020864986,"teacher_disagreement_score":0.020509413,"about_ca_system_score_codex":0.0005061149,"about_ca_system_score_gemma":0.00013997788,"threshold_uncertainty_score":0.040780067},"labels":[],"label_agreement":null},{"id":"W2955653516","doi":"10.3847/1538-4357/ab498b","title":"Can Neutron-star Mergers Explain the r-process Enrichment in Globular Clusters?","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Neutron star; Physics; Globular cluster; Astrophysics; Supernova; Ejecta; Population; Star cluster; r-process; Stars; Astronomy; Nucleosynthesis","score_opus":0.006828622560261866,"score_gpt":0.22511762129284268,"score_spread":0.2182889987325808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955653516","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940528,0.000322941,0.0029140392,0.00029501526,0.000010571402,0.000014632564,0.00006936152,0.000049067185,0.0022716192],"genre_scores_gemma":[0.9992198,0.00009965274,0.00031319066,0.000016619151,0.0000076035353,0.0000035231176,0.000025349711,0.00000742871,0.0003068028],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992037,0.000017976305,0.0000049657815,0.000017848495,0.000014041063,0.000024731708],"domain_scores_gemma":[0.99957687,0.00012425728,0.00013660273,0.0000448143,0.00004107974,0.000076426346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005450701,0.00040731483,0.00035501886,0.0005299119,0.00046692285,0.0006848123,0.00079207553,0.00073998043,0.0011077399],"category_scores_gemma":[0.0015698806,0.00022398627,0.0004519189,0.00042099057,0.0005450402,0.0008165171,0.0007125903,0.00023853511,0.0003585701],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052139215,0.00014583954,0.4894891,0.0001434359,0.00015407693,0.0018629128,0.0007554668,0.43300942,0.01671017,0.04194285,0.0015223512,0.013742917],"study_design_scores_gemma":[0.00007189152,0.00012975407,0.14876048,0.00003085447,0.00007968464,0.00038062176,0.00054596865,0.80749613,0.0030812756,0.036854472,0.0025228453,0.000045967496],"about_ca_topic_score_codex":0.011593296,"about_ca_topic_score_gemma":0.006244661,"teacher_disagreement_score":0.011593296,"about_ca_system_score_codex":0.0011017612,"about_ca_system_score_gemma":0.00039867742,"threshold_uncertainty_score":0.02305162},"labels":[],"label_agreement":null},{"id":"W2955882333","doi":"10.3847/1538-4357/ab2be7","title":"Constraining the Radio Emission of TRAPPIST-1","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Planet; Stars; Astronomy; Exoplanet","score_opus":0.010827630462999647,"score_gpt":0.22185613773589252,"score_spread":0.21102850727289288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2955882333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975878,0.00007865766,0.00052542787,0.000022382523,0.0000041090625,0.000004099238,0.00047578878,0.00004418986,0.0012574949],"genre_scores_gemma":[0.9977539,0.000028372646,0.00088031765,0.000023568185,0.000007972652,0.0000056004974,0.0009883048,0.0000098215705,0.0003022836],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999281,0.00000425407,0.0000021882902,0.000030294732,0.000018278768,0.000016996592],"domain_scores_gemma":[0.9997259,0.000047294456,0.000075389384,0.000027160113,0.000047129848,0.00007715768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012564984,0.0001801075,0.00018769412,0.0005473882,0.00025237483,0.0003422548,0.0002263968,0.00025042993,0.0012806973],"category_scores_gemma":[0.0003113523,0.00013211377,0.00011294429,0.00040571165,0.00013367533,0.00018021675,0.0003017474,0.0002905969,0.000424883],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027838675,0.00008449066,0.7134356,0.000080310456,0.000047407262,0.00039756915,0.0003481287,0.001096647,0.26302287,0.0002563696,0.0012521881,0.019700032],"study_design_scores_gemma":[0.000013799775,0.00019927348,0.97776675,0.000013395446,0.000032740583,0.0005384521,0.00015894588,0.0036361937,0.013933505,0.00012878192,0.0035694987,0.000008641421],"about_ca_topic_score_codex":0.0012623678,"about_ca_topic_score_gemma":0.0031878822,"teacher_disagreement_score":0.0012806973,"about_ca_system_score_codex":0.00019048432,"about_ca_system_score_gemma":0.00008611677,"threshold_uncertainty_score":0.004284382},"labels":[],"label_agreement":null},{"id":"W2956497631","doi":"10.3847/1538-4357/ab2bef","title":"Mass Measurements for Two Binary Pulsars Discovered in the PALFA Survey","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Millisecond pulsar; Pulsar; Binary pulsar; Binary number; Proper motion; Pulsar planet; Binary star; Millisecond","score_opus":0.04108586733019676,"score_gpt":0.35463790303948417,"score_spread":0.3135520357092874,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2956497631","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982316,0.000055331406,0.000232179,0.000011610953,0.0000060545476,0.000005915755,0.00054101716,0.000016642696,0.0008996845],"genre_scores_gemma":[0.9970228,0.00004711331,0.0006885961,0.000006897686,0.000011688518,0.000009884069,0.0018698355,0.000006088086,0.00033707553],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967086,0.000046926332,0.00003204135,0.00008199964,0.00012308572,0.000045087698],"domain_scores_gemma":[0.9984042,0.00018312167,0.0008312408,0.00014133134,0.00027548918,0.00016462721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046020563,0.0002539682,0.00023165371,0.002384262,0.00035125337,0.00040762615,0.0003148198,0.00020724288,0.0013353983],"category_scores_gemma":[0.0016306574,0.0001682326,0.00017185627,0.0011310547,0.00022162104,0.0003245633,0.00065473747,0.0002315517,0.000403672],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018876634,0.000024692536,0.981964,0.000016844884,0.00003320824,0.00014637833,0.00019477347,0.000118341646,0.009615385,0.0001059166,0.00018269307,0.0074090646],"study_design_scores_gemma":[0.00000776256,0.000049715378,0.997334,0.0000019115519,0.000010425801,0.00016827753,0.00006879684,0.00017431405,0.0013479604,0.00002585571,0.00080751616,0.0000034110358],"about_ca_topic_score_codex":0.0026110564,"about_ca_topic_score_gemma":0.0052224835,"teacher_disagreement_score":0.0026110564,"about_ca_system_score_codex":0.0003352977,"about_ca_system_score_gemma":0.00015218633,"threshold_uncertainty_score":0.005191684},"labels":[],"label_agreement":null},{"id":"W2956695507","doi":"10.3847/1538-4357/ab32f1","title":"Stellar and Dust Properties of a Complete Sample of Massive Dusty Galaxies at 1 ≤ <i>z</i> ≤ 4 from MAGPHYS Modeling of UltraVISTA DR3 and <i>Herschel</i> Photometry","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy; Photometry (optics); Star formation; Stellar population; Spectral energy distribution; Cosmic dust; COSMIC cancer database","score_opus":0.013274543264457398,"score_gpt":0.19424559382587211,"score_spread":0.18097105056141471,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2956695507","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977769,0.000021202723,0.0002467826,0.0000078871535,3.0648994e-7,0.0000030565848,0.0016130736,0.000029586288,0.00030118122],"genre_scores_gemma":[0.9933931,0.000024713265,0.0004498803,0.000008779074,0.0000025964084,0.0000059858144,0.005831747,0.000012479411,0.00027059342],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999925,0.000007610985,0.0000042130737,0.000027209444,0.000015126323,0.000020874304],"domain_scores_gemma":[0.9998141,0.000025672054,0.000055695113,0.000039105584,0.000023195933,0.000042267897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013153291,0.00020650869,0.0002301549,0.0005519868,0.0001600596,0.00030744483,0.00033534694,0.00020174704,0.0012122067],"category_scores_gemma":[0.0002552044,0.00013891283,0.0003937597,0.00049009273,0.00008810198,0.00020527859,0.00030503323,0.000110919915,0.00066739495],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010209721,0.000071216775,0.9785653,0.0000127361145,0.000068224486,0.0000857174,0.00014280643,0.0069052037,0.0071114637,0.00017791896,0.0004895855,0.0062678177],"study_design_scores_gemma":[0.0000060277894,0.00002967081,0.98836434,0.0000017289433,0.000015179969,0.0000702581,0.000045639797,0.010002455,0.00068109937,0.00007216429,0.000707352,0.000004010815],"about_ca_topic_score_codex":0.010159727,"about_ca_topic_score_gemma":0.00780952,"teacher_disagreement_score":0.010159727,"about_ca_system_score_codex":0.0003105513,"about_ca_system_score_gemma":0.00011028069,"threshold_uncertainty_score":0.020201206},"labels":[],"label_agreement":null},{"id":"W2958258857","doi":"10.3847/1538-4357/ab46b9","title":"Analysis of Helium-rich White Dwarfs Polluted by Heavy Elements in the Gaia Era","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":128,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"White dwarf; Stars; Photometry (optics); Sky; Parallax; Stellar classification; Main sequence; Spectral line","score_opus":0.006667729399459177,"score_gpt":0.22643628261687224,"score_spread":0.21976855321741307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2958258857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99797493,0.00014261014,0.00013801054,0.000010956714,0.0000013402898,0.0000051324005,0.0011864265,0.000018204862,0.00052237953],"genre_scores_gemma":[0.9964592,0.000075645985,0.00019824343,0.000010642161,0.0000030721646,0.0000029495059,0.002767175,0.0000076097444,0.00047555176],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998652,0.000009682898,0.000006916934,0.00003511279,0.000046836903,0.000036265727],"domain_scores_gemma":[0.9996482,0.000022938792,0.000097212134,0.000026118243,0.00009486925,0.00011063934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017635475,0.0002294098,0.00029558432,0.0023369272,0.00042002072,0.0005065676,0.0002526888,0.00010652614,0.0007282978],"category_scores_gemma":[0.0004083262,0.00008121378,0.00019656032,0.0017899233,0.00018452134,0.00012603996,0.0004714116,0.00009161736,0.00023695969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005777813,0.000008031547,0.9908189,0.000009555997,0.00003194206,0.00010544425,0.000097235345,0.00015136332,0.00543983,0.000052962478,0.00021537124,0.0030116048],"study_design_scores_gemma":[9.963662e-7,0.000007542994,0.9988105,0.0000010048427,0.00000774141,0.00003658372,0.000053087104,0.00017025971,0.00045560472,0.0000071107493,0.00044831075,0.0000012598588],"about_ca_topic_score_codex":0.15459436,"about_ca_topic_score_gemma":0.2451682,"teacher_disagreement_score":0.15459436,"about_ca_system_score_codex":0.00082903175,"about_ca_system_score_gemma":0.00039322663,"threshold_uncertainty_score":0.30738902},"labels":[],"label_agreement":null},{"id":"W2960284535","doi":"10.3847/1538-4357/ab3049","title":"Space Telescope and Optical Reverberation Mapping Project. VIII. Time Variability of Emission and Absorption in NGC 5548 Based on Modeling the Ultraviolet Spectrum","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Smithsonian Astrophysical Observatory; University of California, Santa Barbara; Jet Propulsion Laboratory; Nederlandse Onderzoekschool Voor Astronomie; National Research Foundation of Korea; Nuclear Safety and Security Commission; Science and Technology Facilities Council; National Research Foundation; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Space Telescope Science Institute; Ohio State University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Georgia State University; California Institute of Technology; National Aeronautics and Space Administration; Howard Hughes Medical Institute; David and Lucile Packard Foundation; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; Smithsonian Institution; Danmarks Frie Forskningsfond; National Science Foundation","keywords":"Galaxy; Emission spectrum; Reverberation mapping; Absorption (acoustics); Spectral line; Absorption spectroscopy; Active galactic nucleus; Equivalent width; Ultraviolet","score_opus":0.006552035235639917,"score_gpt":0.20612415444293142,"score_spread":0.1995721192072915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2960284535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889658,0.00005714956,0.0054109357,0.00010038883,0.00001605388,0.00002340408,0.0028126366,0.0003236758,0.0022899986],"genre_scores_gemma":[0.99230725,0.000036979334,0.0031834661,0.00001800784,0.0000083583855,0.000019929706,0.0028379986,0.000043550997,0.0015445072],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992514,0.000014371309,0.0000023170549,0.000023666144,0.000015148672,0.000019361556],"domain_scores_gemma":[0.9998349,0.000019538948,0.000049180722,0.000036087677,0.00003569572,0.000024557023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025442793,0.0004092722,0.00019203807,0.00032253674,0.0001676246,0.0003934004,0.00043958286,0.00033148334,0.0015426493],"category_scores_gemma":[0.0005386308,0.00015036008,0.000436676,0.0002270516,0.00012408625,0.0003769008,0.00019847523,0.00020092636,0.0004935316],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004254458,0.00017640673,0.3490462,0.000059864447,0.00015650531,0.00035500238,0.0002067858,0.60979664,0.010319343,0.0016152676,0.0046343715,0.023208117],"study_design_scores_gemma":[0.000054573047,0.00017178354,0.2116366,0.000010992704,0.00005079602,0.00012881364,0.000062992374,0.77904373,0.0031027438,0.0010455645,0.004664754,0.000026729844],"about_ca_topic_score_codex":0.04158195,"about_ca_topic_score_gemma":0.02797105,"teacher_disagreement_score":0.04158195,"about_ca_system_score_codex":0.00074646744,"about_ca_system_score_gemma":0.0002566886,"threshold_uncertainty_score":0.08267987},"labels":[],"label_agreement":null},{"id":"W2961226542","doi":"10.3847/1538-4357/ab32ea","title":"Thermal Infrared Imaging of MWC 758 with the Large Binocular Telescope: Planetary-driven Spiral Arms?","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Planet; Astrophysics; Spiral galaxy; Spiral (railway); Astronomy; Telescope; Brightness; Logarithmic spiral; Giant planet; Planetary system; Stars; Geometry","score_opus":0.004986262864135372,"score_gpt":0.19568385178371622,"score_spread":0.19069758891958086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2961226542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99682367,0.00009131094,0.00046650675,0.000056119523,0.000004285872,0.000005070525,0.0002736006,0.000037164154,0.0022423472],"genre_scores_gemma":[0.99912184,0.000018545506,0.00041022428,0.00002305256,0.0000051012985,0.0000022166712,0.00013992083,0.0000032791158,0.0002758087],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999938,0.0000026703558,0.0000025081174,0.000015754913,0.0000163102,0.000024711682],"domain_scores_gemma":[0.99981314,0.0000149631705,0.000047789308,0.000019516623,0.00002610313,0.00007856172],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012459727,0.00015831963,0.00018474564,0.0007530783,0.00027030695,0.00040314128,0.00024964585,0.00019776796,0.0016921093],"category_scores_gemma":[0.00023731105,0.0001226306,0.00014273137,0.00037397703,0.00018043134,0.00025657652,0.0003940781,0.00017516573,0.00023017378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028411776,0.00008298435,0.5488291,0.00007977126,0.00007923151,0.0015451391,0.00054423575,0.00038446442,0.4225289,0.00036985046,0.0010716169,0.024200581],"study_design_scores_gemma":[0.000009771055,0.000056522735,0.9904,0.00000781627,0.000031049563,0.0005005618,0.00021862928,0.0008309037,0.0067240587,0.00008779738,0.0011256894,0.000007198062],"about_ca_topic_score_codex":0.005097859,"about_ca_topic_score_gemma":0.017544791,"teacher_disagreement_score":0.005097859,"about_ca_system_score_codex":0.0003319612,"about_ca_system_score_gemma":0.00014609963,"threshold_uncertainty_score":0.010136366},"labels":[],"label_agreement":null},{"id":"W2961798372","doi":"10.3847/1538-4357/ab31f3","title":"The Kennicutt–Schmidt Law and Gas Scale Height in Luminous and Ultraluminous Infrared Galaxies","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Inverse; Star formation; Luminous infrared galaxy; Infrared; Velocity dispersion; Line (geometry); Turbulence; Millimeter; Thermodynamics; Optics; Geometry","score_opus":0.004290601427566917,"score_gpt":0.20166327707273343,"score_spread":0.19737267564516653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2961798372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917563,0.00066111964,0.004371493,0.00009860768,0.00000773505,0.000004339702,0.00017496197,0.00011332542,0.0028122263],"genre_scores_gemma":[0.9985544,0.000097787226,0.0008564557,0.000015039424,0.000012878374,0.0000031572997,0.00022513434,0.000013337604,0.00022184465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998286,0.000018669198,0.0000073721067,0.000049634204,0.000053268726,0.000042439286],"domain_scores_gemma":[0.99886453,0.00024138756,0.00039585689,0.00013612061,0.000104365,0.00025781314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034180642,0.00020615438,0.00019737218,0.001502096,0.00026023507,0.0006394501,0.0003633676,0.00023863043,0.0006224761],"category_scores_gemma":[0.0015640507,0.00018965248,0.0003198433,0.0011196384,0.0011657109,0.00062540954,0.00046631013,0.00051893573,0.0002562389],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018681455,0.000044279812,0.9308844,0.000026327201,0.0001240866,0.0002612789,0.0006816196,0.0064679184,0.011721357,0.013014281,0.0016293563,0.034958344],"study_design_scores_gemma":[0.0000047608287,0.00001123755,0.9900384,0.0000035316978,0.000005791666,0.00008720973,0.00007999846,0.0050252117,0.0006625594,0.003332176,0.00073706475,0.000012162699],"about_ca_topic_score_codex":0.011076213,"about_ca_topic_score_gemma":0.0076600043,"teacher_disagreement_score":0.011076213,"about_ca_system_score_codex":0.0008004691,"about_ca_system_score_gemma":0.00017976745,"threshold_uncertainty_score":0.022023499},"labels":[],"label_agreement":null},{"id":"W2962647378","doi":"10.3847/1538-4357/ab3226","title":"Dust Destruction in Nonradiative Shocks","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"National Natural Science Foundation of China; National Key Research and Development Program of China; National Aeronautics and Space Administration","keywords":"Interstellar medium; Cosmic dust; Shock wave; Interstellar cloud; Intergalactic dust; Astrochemistry; Extinction (optical mineralogy)","score_opus":0.007681817171426481,"score_gpt":0.23000314212572706,"score_spread":0.22232132495430057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962647378","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99949586,0.00014220635,0.000064626205,0.0000017230204,5.785006e-7,0.0000012335591,0.000036018853,0.0000026406608,0.00025513134],"genre_scores_gemma":[0.9996991,0.000041978317,0.00003172372,0.0000016570872,9.24811e-7,5.736065e-7,0.000059943533,9.966251e-7,0.00016313918],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985063,0.000013811106,0.000014960422,0.000035934554,0.00004458301,0.000040055143],"domain_scores_gemma":[0.9996203,0.00005100304,0.00018676501,0.00004160068,0.000042445867,0.000057840938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016201088,0.00014168007,0.00019101758,0.0005790753,0.00019171133,0.0003630418,0.00017946669,0.00012623446,0.00089806295],"category_scores_gemma":[0.00036166227,0.00007354658,0.00016103551,0.00026742162,0.00025063058,0.0001825484,0.00042423708,0.00009592617,0.00015304505],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072457164,0.00004682996,0.8614351,0.00007230319,0.00009939054,0.00058416656,0.0002397665,0.0019024746,0.12339918,0.00020183434,0.000062591585,0.011231706],"study_design_scores_gemma":[0.0000044820918,0.00009527974,0.98356414,0.0000022280606,0.0000114432505,0.00032395715,0.00011548129,0.0005124564,0.015028042,0.00008192428,0.00025792918,0.000002544986],"about_ca_topic_score_codex":0.0018515246,"about_ca_topic_score_gemma":0.0015354413,"teacher_disagreement_score":0.0018515246,"about_ca_system_score_codex":0.00030166196,"about_ca_system_score_gemma":0.0000856333,"threshold_uncertainty_score":0.0036814213},"labels":[],"label_agreement":null},{"id":"W2962887298","doi":"10.3847/0004-637x/820/2/116","title":"THE Fe II EMISSION IN ACTIVE GALACTIC NUCLEI: EXCITATION MECHANISMS AND LOCATION OF THE EMITTING REGION","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Active galactic nucleus; Astrophysics; Excitation; Flux (metallurgy); Line (geometry); Fluorescence; Doubly ionized oxygen; Near-infrared spectroscopy; Emission spectrum; Atomic physics; Spectral line; Galaxy; Astronomy; Optics; Chemistry","score_opus":0.007302626111715216,"score_gpt":0.20865543186909047,"score_spread":0.20135280575737524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962887298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990721,0.00018628736,0.00030465686,0.000002213895,5.678529e-7,0.0000031268446,0.000068155736,0.0000054370807,0.00035740505],"genre_scores_gemma":[0.99960965,0.000040483774,0.00017523326,0.000001917074,7.1939655e-7,0.0000019445094,0.00008478601,0.0000016143874,0.000083677],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999244,0.000010776373,0.000004787987,0.000025928233,0.000018885708,0.0000152893],"domain_scores_gemma":[0.9998536,0.000029551438,0.000049256367,0.000014649546,0.000024344077,0.000028658002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013229693,0.00020612236,0.00018666791,0.00039669257,0.00014630679,0.00030531661,0.0002607243,0.00023588401,0.00046829128],"category_scores_gemma":[0.0002965986,0.00010318258,0.00016983807,0.00025137461,0.00016917878,0.0001492892,0.00010595325,0.00010120576,0.00018715908],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038593815,0.000115395065,0.6294113,0.00005273713,0.000082981234,0.00022703738,0.00011848372,0.0023323498,0.36086944,0.00010410442,0.00004069978,0.006259602],"study_design_scores_gemma":[0.0000059263566,0.0001204147,0.97299474,0.000004139971,0.000031853233,0.00028179726,0.000090417925,0.0022817408,0.023894526,0.000053970824,0.00023559194,0.000004776867],"about_ca_topic_score_codex":0.0041106185,"about_ca_topic_score_gemma":0.0033856314,"teacher_disagreement_score":0.0041106185,"about_ca_system_score_codex":0.00023130172,"about_ca_system_score_gemma":0.00006803535,"threshold_uncertainty_score":0.0081733465},"labels":[],"label_agreement":null},{"id":"W2962891736","doi":"10.3847/1538-4357/ab0e6d","title":"A Multimass Velocity Dispersion Model of 47 Tucanae Indicates No Evidence for an Intermediate-mass Black Hole","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":172,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Velocity dispersion; Black hole (networking); Mass segregation; Stars; Intermediate-mass black hole; Stellar mass; Star cluster; Stellar collision; Blue straggler; Stellar dynamics; Photometry (optics); Binary black hole; Stellar black hole; Astronomy; Stellar evolution; Star formation; Galaxy","score_opus":0.0353416699929843,"score_gpt":0.2809397964343605,"score_spread":0.2455981264413762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962891736","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947373,0.00004365286,0.0033610486,0.00009593208,0.000007279495,0.000008246098,0.00012700164,0.000041969135,0.0015775311],"genre_scores_gemma":[0.99873704,0.0000140517295,0.0003602841,0.000012816447,0.0000032828711,0.000004825144,0.000110389105,0.000010392962,0.0007469248],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986017,0.000012890837,0.000003740152,0.000043011933,0.000018509612,0.00006171683],"domain_scores_gemma":[0.9997311,0.00004519999,0.000048529153,0.000027690292,0.000059390077,0.000088094865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032551092,0.00041678757,0.00056790595,0.00072842033,0.0012185727,0.0011679122,0.0017296631,0.00085518125,0.0021805242],"category_scores_gemma":[0.0007810449,0.0002744884,0.00056922546,0.00050762546,0.00084734376,0.0005644181,0.0005547511,0.00048561202,0.00028124114],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031843188,0.00011021631,0.12558703,0.000020867612,0.00013516625,0.00038264884,0.00028582348,0.84983677,0.006696375,0.009660744,0.000900568,0.006065341],"study_design_scores_gemma":[0.000029504765,0.000030973675,0.033640508,0.0000054219845,0.000030288105,0.000041019994,0.00010293089,0.9636728,0.00050738285,0.0014459178,0.00046962473,0.000023646911],"about_ca_topic_score_codex":0.30107516,"about_ca_topic_score_gemma":0.14397395,"teacher_disagreement_score":0.30107516,"about_ca_system_score_codex":0.0031999012,"about_ca_system_score_gemma":0.0014814326,"threshold_uncertainty_score":0.59864545},"labels":[],"label_agreement":null},{"id":"W2962953922","doi":"10.3847/1538-4357/ab264b","title":"The Atacama Cosmology Telescope: CO(J = 3 – 2) Mapping and Lens Modeling of an ACT-selected Dusty Star-forming Galaxy","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Galaxy; Gravitational lens; Telescope; Cosmology; Luminosity; Line (geometry); Brightness; Brightness temperature","score_opus":0.014490211280165107,"score_gpt":0.24134484497043365,"score_spread":0.22685463369026854,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2962953922","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969478,0.000049962247,0.0019650047,0.000030755968,0.0000017885991,0.000004738645,0.00014433044,0.000055041768,0.0008005865],"genre_scores_gemma":[0.998302,0.0000138297255,0.0014509837,0.000006402956,0.0000020321625,0.0000017820106,0.00009089069,0.000011613987,0.000120408535],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999948,0.000009527651,0.0000020698187,0.000018476829,0.000010190075,0.000011848323],"domain_scores_gemma":[0.99978083,0.000032515873,0.00006515407,0.000027544305,0.00003867986,0.000055147877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022572883,0.0002078835,0.00013089742,0.00041382018,0.00025649872,0.000507092,0.0003495477,0.00023081263,0.0005739171],"category_scores_gemma":[0.00036483674,0.0001402804,0.00025111737,0.00041012594,0.00015786529,0.00021441148,0.00024377357,0.00014237917,0.0001355544],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039921276,0.00010613441,0.7589435,0.000047285703,0.00020801941,0.00052500254,0.00032804225,0.17048553,0.046676476,0.002868532,0.0013062247,0.018105973],"study_design_scores_gemma":[0.000021872393,0.0000293782,0.47964072,0.00000439636,0.000032111293,0.000083447,0.00008727639,0.51615363,0.0025644244,0.00056793273,0.00080047216,0.000014354488],"about_ca_topic_score_codex":0.049451217,"about_ca_topic_score_gemma":0.03873077,"teacher_disagreement_score":0.049451217,"about_ca_system_score_codex":0.00093376834,"about_ca_system_score_gemma":0.00033766348,"threshold_uncertainty_score":0.0983268},"labels":[],"label_agreement":null},{"id":"W2963018017","doi":"10.1088/0004-637x/806/2/210","title":"ULTRAVIOLET/X-RAY VARIABILITY AND THE EXTENDED X-RAY EMISSION OF THE RADIO-LOUD BROAD ABSORPTION LINE QUASAR PG 1004+130","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Quasar; Astrophysics; Line-of-sight; X-ray; Astronomy; Absorption (acoustics); Emission spectrum; Spectral line; Active galactic nucleus; Galaxy; Ultraviolet; Optics","score_opus":0.014921633827199111,"score_gpt":0.24118968325372925,"score_spread":0.22626804942653014,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963018017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989121,0.000045071356,0.00010251235,0.0000109771745,0.0000012364642,0.0000017202527,0.00019410915,0.000012912261,0.0007193188],"genre_scores_gemma":[0.9989593,0.000053903164,0.00020585346,0.000011253669,0.000007965273,0.00000324474,0.00053216144,0.0000047724484,0.00022166767],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999515,0.000005176547,0.000002088108,0.000014610265,0.000013069969,0.000013447444],"domain_scores_gemma":[0.9997143,0.000040556763,0.0001449405,0.000026113545,0.000015555399,0.000058496724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011544368,0.00016141092,0.00010874023,0.0007479321,0.00013051082,0.00036498602,0.00018263319,0.00014975142,0.0010659595],"category_scores_gemma":[0.00030329678,0.00010499946,0.00013359607,0.00048281634,0.00025359847,0.0002467026,0.0004124978,0.00024171743,0.00018368821],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019247238,0.00010972207,0.9482027,0.000035665114,0.00008815869,0.00037667342,0.00017103445,0.00083447597,0.038952235,0.00015303642,0.00032153327,0.010562315],"study_design_scores_gemma":[0.0000017809092,0.000025805359,0.99915326,0.0000011807554,0.000007490904,0.00011569715,0.000022118113,0.00016061855,0.00030667268,0.000027150692,0.00017637537,0.000001694528],"about_ca_topic_score_codex":0.0023975908,"about_ca_topic_score_gemma":0.005132891,"teacher_disagreement_score":0.0023975908,"about_ca_system_score_codex":0.0001691804,"about_ca_system_score_gemma":0.0000691643,"threshold_uncertainty_score":0.0047672987},"labels":[],"label_agreement":null},{"id":"W2963157964","doi":"10.1088/0004-637x/814/2/96","title":"THE STAR FORMATION HISTORY OF BCGs TO<i>z</i>= 1.8 FROM THE SpARCS/SWIRE SURVEY: EVIDENCE FOR SIGNIFICANT IN SITU STAR FORMATION AT HIGH REDSHIFT","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University","funders":"Lawrence Berkeley National Laboratory; York University; Space Telescope Science Institute; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Redshift; Star formation; Galaxy; Astronomy; Stellar mass; Luminosity; Population; Photometric redshift; Stellar population","score_opus":0.04225777512173736,"score_gpt":0.24354343505225082,"score_spread":0.20128565993051345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963157964","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995807,0.000041902793,0.000019142333,0.000008626126,7.2192336e-7,0.0000015919765,0.00020789859,0.0000032092692,0.00013626654],"genre_scores_gemma":[0.99894327,0.000034004377,0.00006461155,0.000012078794,0.0000039250617,0.0000017582412,0.0008562159,0.000002017445,0.00008209656],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984264,0.000015821252,0.00001095437,0.000043297492,0.00003650423,0.000050737148],"domain_scores_gemma":[0.99889,0.00008521562,0.0004101115,0.00007725177,0.0001371063,0.00040045887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003210115,0.00013985408,0.00022022912,0.0010468159,0.0002960934,0.00037585202,0.00025313924,0.0001990341,0.0008084283],"category_scores_gemma":[0.0008235572,0.00012955755,0.00014781619,0.00047907274,0.00024737412,0.0002191326,0.00038942823,0.0002557298,0.00025817179],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004014532,0.000021543028,0.9961616,0.00000540364,0.000017039012,0.000031354666,0.00015736066,0.0000386388,0.002166944,0.000017912334,0.00010841212,0.0012336577],"study_design_scores_gemma":[7.192083e-7,0.000010263766,0.9998047,6.843819e-7,0.0000031759753,0.00002761698,0.000021819033,0.000026282458,0.000053802913,0.0000020967982,0.000048434606,4.7419178e-7],"about_ca_topic_score_codex":0.011840382,"about_ca_topic_score_gemma":0.021141632,"teacher_disagreement_score":0.011840382,"about_ca_system_score_codex":0.00023610903,"about_ca_system_score_gemma":0.00015403594,"threshold_uncertainty_score":0.023542881},"labels":[],"label_agreement":null},{"id":"W2963186413","doi":"10.3847/1538-4357/ab23ff","title":"The East Asian Observatory SCUBA-2 Survey of the COSMOS Field: Unveiling 1147 Bright Sub-millimeter Sources across 2.6 Square Degrees","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; McMaster University; Dalhousie University","funders":"Japan Society for the Promotion of Science; Canadian Space Agency; East Asian Core Observatories Association; Narodowym Centrum Nauki; Korea Astronomy and Space Science Institute; Chinese Academy of Sciences; Academia Sinica; Science and Technology Facilities Council; National Astronomical Observatory of Japan; European Commission","keywords":"Physics; Cosmic variance; James Clerk Maxwell Telescope; Astrophysics; Galaxy; Redshift; Observatory; RADIUS; Bulge; Telescope; Sigma; Effective radius; Astronomy; Star formation","score_opus":0.01347332613013729,"score_gpt":0.2236357091978726,"score_spread":0.2101623830677353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963186413","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973768,0.00014172998,0.00034227702,0.00001599244,0.000002505724,0.000006877214,0.0012732114,0.00004047216,0.0008002278],"genre_scores_gemma":[0.99524885,0.00012321224,0.0009251611,0.000026442154,0.000016883017,0.000010111293,0.0032851335,0.000014546257,0.00034973133],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999838,0.00001942243,0.000012891595,0.00004582203,0.000049471495,0.000034407538],"domain_scores_gemma":[0.999226,0.00006444206,0.00022903304,0.0001460477,0.00012998053,0.00020452982],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031200633,0.00032905734,0.00023640209,0.0020522166,0.00036961937,0.00054396404,0.00026725925,0.00015791603,0.0013709455],"category_scores_gemma":[0.00040230493,0.00021015001,0.00027091714,0.0019595379,0.00017859813,0.00031949283,0.0007834104,0.00018809276,0.0004182491],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001496758,0.000060781393,0.9681075,0.000032104464,0.000114733164,0.00018388557,0.0002207595,0.0006382888,0.01531672,0.00017168174,0.0014042001,0.013599704],"study_design_scores_gemma":[0.0000054763877,0.000014311888,0.99770516,0.0000053366202,0.000018658924,0.000057100442,0.00008773375,0.0005511934,0.0008125584,0.000023974027,0.0007141695,0.000004233851],"about_ca_topic_score_codex":0.008315523,"about_ca_topic_score_gemma":0.01878766,"teacher_disagreement_score":0.008315523,"about_ca_system_score_codex":0.0001693867,"about_ca_system_score_gemma":0.00027853905,"threshold_uncertainty_score":0.016534269},"labels":[],"label_agreement":null},{"id":"W2963197133","doi":"10.3847/1538-4357/aa9f1a","title":"Hydrogen-poor Superluminous Supernovae from the Pan-STARRS1 Medium Deep Survey","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":116,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; FAS Division of Science, Harvard University; National Aeronautics and Space Administration; Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Harvard University; Queen's University; Ministerio de Ciencia, Tecnología e Innovación Productiva; Deutsche Forschungsgemeinschaft; Eötvös Loránd Tudományegyetem; European Commission; Munich Institute for Astro- and Particle Physics; Los Alamos National Laboratory; Alfred P. Sloan Foundation; Johns Hopkins University; National Central University; Queen's University Belfast; Gordon and Betty Moore Foundation; Space Telescope Science Institute; Smithsonian Institution; Durham University; Ministério da Ciência, Tecnologia e Inovação; National Science Foundation","keywords":"Light curve; Redshift; Luminosity; Supernova; Spectral line; Cosmology; Range (aeronautics); Emission spectrum","score_opus":0.01606293721208589,"score_gpt":0.23425889806849956,"score_spread":0.21819596085641368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963197133","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99666095,0.00008477592,0.0001441218,0.000019329591,0.00000202484,0.000006438605,0.0023166905,0.000039229813,0.0007263984],"genre_scores_gemma":[0.9908903,0.00011619565,0.0004243076,0.000016729406,0.00000800297,0.000009318379,0.008066505,0.000015851414,0.0004527875],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979633,0.000026374059,0.00001778966,0.00004995542,0.0000604599,0.000049158472],"domain_scores_gemma":[0.99899393,0.000088862165,0.0003817796,0.00014046616,0.00014447379,0.00025052766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049301813,0.00031425332,0.0002806457,0.0019540826,0.0002740201,0.00050381914,0.00024901069,0.0001295158,0.0017332202],"category_scores_gemma":[0.0009609162,0.0001382757,0.00024294012,0.0009753723,0.00015786091,0.00030631493,0.00085557,0.0001728802,0.00057184196],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000107797154,0.000018148474,0.9847147,0.000036311536,0.000062000174,0.00007213565,0.00012911182,0.00022134725,0.0047738063,0.000075821335,0.0007476628,0.009041214],"study_design_scores_gemma":[0.0000025597774,0.000020199137,0.99785763,0.0000040659324,0.000010039353,0.00015528116,0.000069856666,0.00016982174,0.00059279293,0.000020457928,0.001094878,0.0000025396341],"about_ca_topic_score_codex":0.0037751535,"about_ca_topic_score_gemma":0.008882754,"teacher_disagreement_score":0.0037751535,"about_ca_system_score_codex":0.00021058791,"about_ca_system_score_gemma":0.00016113381,"threshold_uncertainty_score":0.0075063705},"labels":[],"label_agreement":null},{"id":"W2963270007","doi":"10.3847/1538-4357/aa8309","title":"Spectral Sequences of Type Ia Supernovae. I. Connecting Normal and Subluminous SNe Ia and the Presence of Unburned Carbon","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Ejecta; Supernova; Astrophysics; Physics; White dwarf; Spectral line; Type (biology); Carbon fibers; Luminosity; Astronomy; Materials science; Geology; Stars","score_opus":0.014002473324578879,"score_gpt":0.25280652441242707,"score_spread":0.2388040510878482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963270007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965739,0.000098597826,0.0005328202,0.000019511435,0.000006402225,0.000011961228,0.00052015827,0.000034961147,0.0022017634],"genre_scores_gemma":[0.9978865,0.000033565746,0.0005525268,0.000012237667,0.000005639157,0.000007949757,0.0012117592,0.000007877005,0.00028202793],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998741,0.000018441102,0.000021675405,0.0000321965,0.0000291417,0.00002441414],"domain_scores_gemma":[0.9982799,0.00031629496,0.0005391322,0.00011599767,0.0003028112,0.00044582883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031828342,0.00019532183,0.00012680619,0.0016879644,0.00028369072,0.0004948178,0.00020277436,0.0003438024,0.0020746437],"category_scores_gemma":[0.0013909023,0.00012326591,0.00023805027,0.00049385417,0.00024312062,0.0002668305,0.00041288018,0.0002457476,0.00040470154],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049965386,0.00009150066,0.9676664,0.000027646793,0.00004261877,0.00020164548,0.0001271881,0.0011447623,0.018920038,0.0006385787,0.00035571758,0.010284204],"study_design_scores_gemma":[0.000004345515,0.000067886875,0.99700886,0.000003574292,0.0000073910687,0.00031338228,0.00007787277,0.0011402534,0.0008453566,0.0002606888,0.00026679094,0.000003657121],"about_ca_topic_score_codex":0.0017039948,"about_ca_topic_score_gemma":0.0025742732,"teacher_disagreement_score":0.0020746437,"about_ca_system_score_codex":0.00027321742,"about_ca_system_score_gemma":0.00011431103,"threshold_uncertainty_score":0.0069403052},"labels":[],"label_agreement":null},{"id":"W2963374686","doi":"10.3847/1538-4357/aa89e7","title":"Halo Nonlinear Reconstruction","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; Canadian Institute for Advanced Research","funders":"","keywords":"Halo; Redshift; Astrophysics; Physics; Scale (ratio); Sample (material); Nonlinear system; Computational physics; Galaxy; Quantum mechanics","score_opus":0.009511244287576742,"score_gpt":0.2254687347526151,"score_spread":0.21595749046503837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963374686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6135871,0.00018756503,0.36240473,0.0008415061,0.00009159069,0.000100316975,0.0019198637,0.0025386515,0.018328764],"genre_scores_gemma":[0.9471115,0.000056489374,0.047339924,0.00009264358,0.000018260722,0.00002805921,0.0009577891,0.00032388378,0.004071456],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998066,0.00005148796,0.0000073978267,0.000031974447,0.00005459304,0.000047979243],"domain_scores_gemma":[0.9992217,0.00023875305,0.00006955814,0.00015507122,0.00024814176,0.000066740664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006599919,0.00038336377,0.00032238054,0.0005145187,0.00032428713,0.0007249007,0.0007385623,0.00062047195,0.005536958],"category_scores_gemma":[0.0032646568,0.00027078003,0.00050293515,0.00051469554,0.00045221002,0.00049280905,0.00082099775,0.00049673714,0.00079817604],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037035256,0.00006359449,0.009008894,0.0000723368,0.00006247345,0.00018841239,0.0001029372,0.9429372,0.0058168895,0.009682669,0.0024664414,0.029227883],"study_design_scores_gemma":[0.000014496862,0.000010356508,0.0008253575,0.0000030728324,0.0000027169708,0.000027870483,0.000012904884,0.99606663,0.0014568036,0.0012186116,0.00035446964,0.000006624632],"about_ca_topic_score_codex":0.01743683,"about_ca_topic_score_gemma":0.011049252,"teacher_disagreement_score":0.01743683,"about_ca_system_score_codex":0.0006504234,"about_ca_system_score_gemma":0.00088962,"threshold_uncertainty_score":0.03467065},"labels":[],"label_agreement":null},{"id":"W2963437138","doi":"10.3847/1538-4357/ab1f83","title":"Differences in Faraday Rotation between Adjacent Extragalactic Radio Sources as a Probe of Cosmic Magnetic Fields","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Faraday effect; COSMIC cancer database; Astronomy; Magnetic field; Astrophysics; Rotation (mathematics); Faraday cage","score_opus":0.0090214781663182,"score_gpt":0.21337809813384603,"score_spread":0.20435661996752782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963437138","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99682045,0.00007300889,0.00049279723,0.000017806537,0.0000043174914,0.000004151204,0.0005781074,0.000015146609,0.001994153],"genre_scores_gemma":[0.99887556,0.000020013147,0.00020860364,0.000008024608,0.000006522716,0.0000030956094,0.0007129357,0.0000035247801,0.00016167427],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996055,0.00011485193,0.000026962265,0.00010321134,0.000097356875,0.000052202508],"domain_scores_gemma":[0.99771726,0.00046726174,0.0009095917,0.00034572146,0.00026730663,0.00029287644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005282331,0.00019022115,0.00021979614,0.0015169574,0.00019931553,0.00046001948,0.00022862632,0.00015241012,0.0018942514],"category_scores_gemma":[0.002580304,0.00009516748,0.00013935528,0.0011062257,0.0002315941,0.0002722431,0.00049464684,0.0001774735,0.0004572588],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039708324,0.000011641784,0.9946913,0.0000069426296,0.000036676523,0.000017913517,0.00006220558,0.00014084498,0.0013337911,0.00008812954,0.00014875371,0.003422032],"study_design_scores_gemma":[0.0000011790829,0.000007810155,0.99955803,0.0000010491761,0.0000035208263,0.000019767958,0.000048130074,0.000076912445,0.00011618163,0.00003203883,0.00013452291,8.493944e-7],"about_ca_topic_score_codex":0.0022835115,"about_ca_topic_score_gemma":0.0034600282,"teacher_disagreement_score":0.0022835115,"about_ca_system_score_codex":0.00017961324,"about_ca_system_score_gemma":0.00007169982,"threshold_uncertainty_score":0.0063369274},"labels":[],"label_agreement":null},{"id":"W2963474097","doi":"10.3847/1538-4357/aa9d88","title":"The Bulge Metallicity Distribution from the APOGEE Survey","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Metallicity; Bulge; Astrophysics; Physics; Milky Way; Galactic Center; Disc; Stars; Thick disk; Astronomy; Population; Stellar population; Thin disk; Red clump; Galaxy; Galaxy formation and evolution; Star formation; Halo","score_opus":0.017237877611496946,"score_gpt":0.2371245844781695,"score_spread":0.21988670686667255,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963474097","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955107,0.0001266051,0.0000756207,0.000033003424,0.0000027256742,0.000002957701,0.0032526664,0.000016832035,0.0009788161],"genre_scores_gemma":[0.9946037,0.000079522004,0.0000747529,0.000016768543,0.000006299993,0.0000032617916,0.0047127903,0.000006447935,0.0004964071],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983525,0.0000166223,0.000010393749,0.000058996346,0.000043250704,0.000035524678],"domain_scores_gemma":[0.99946076,0.000043466935,0.00017542065,0.00006554753,0.00010879606,0.00014612883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021157991,0.00017704385,0.00017279484,0.0018177277,0.0002192996,0.0005012302,0.00017761231,0.00018537433,0.0020491788],"category_scores_gemma":[0.000554491,0.000086962384,0.00011640194,0.00081790047,0.00020826401,0.00027117814,0.0007288856,0.00016152332,0.00043861425],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004078398,0.000007685236,0.9959508,0.0000059215768,0.000029580566,0.000020353511,0.00006452689,0.00007485921,0.00051360397,0.000048650814,0.0006595783,0.002583659],"study_design_scores_gemma":[0.0000011271136,0.0000030515419,0.9996567,0.000001117758,0.0000020637567,0.000013627968,0.000031924927,0.000036196045,0.000031271546,0.0000075096027,0.00021487876,5.926927e-7],"about_ca_topic_score_codex":0.014025297,"about_ca_topic_score_gemma":0.013273969,"teacher_disagreement_score":0.014025297,"about_ca_system_score_codex":0.0002573264,"about_ca_system_score_gemma":0.00009540791,"threshold_uncertainty_score":0.027887344},"labels":[],"label_agreement":null},{"id":"W2963530597","doi":"10.1088/0004-637x/814/1/79","title":"BANGS AND METEORS FROM THE QUIET COMET 15P/FINLAY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Western University","funders":"","keywords":"Physics; Meteor (satellite); Ejecta; Meteoroid; Meteor shower; Astrophysics; Astronomy; Comet; Supernova","score_opus":0.015789775261186724,"score_gpt":0.21625340580390212,"score_spread":0.2004636305427154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963530597","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907494,0.00006187254,0.000026512613,0.00001111952,0.0000027111266,0.000003572113,0.00032364958,0.00000859987,0.00048695868],"genre_scores_gemma":[0.9988096,0.000025211022,0.00008543098,0.000010733471,0.0000035052226,0.0000014339341,0.0008809928,0.0000033343404,0.00017974267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999181,0.0000044604835,0.000004746598,0.000021886452,0.000027076258,0.00002370725],"domain_scores_gemma":[0.99969506,0.000025256993,0.00011164661,0.000020980617,0.000034445522,0.00011260804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018130586,0.00027078777,0.0002304575,0.0007876851,0.00052448787,0.00052481744,0.00020826003,0.00023539759,0.0007020737],"category_scores_gemma":[0.00026483787,0.00013279871,0.00027377415,0.00039219763,0.00022692305,0.00016885952,0.0003822063,0.00020138573,0.00013611575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005444104,0.000071011375,0.9569342,0.00005706751,0.00011727429,0.002323213,0.00054576877,0.0008942974,0.032133836,0.00013285485,0.0007098585,0.0055361018],"study_design_scores_gemma":[0.000003089408,0.00003260547,0.9984119,0.0000029914825,0.0000097935235,0.00015817888,0.000104465136,0.00023568067,0.00070872135,0.000008943889,0.00031934946,0.0000041979215],"about_ca_topic_score_codex":0.042197686,"about_ca_topic_score_gemma":0.075402305,"teacher_disagreement_score":0.042197686,"about_ca_system_score_codex":0.0007728825,"about_ca_system_score_gemma":0.00023911509,"threshold_uncertainty_score":0.08390409},"labels":[],"label_agreement":null},{"id":"W2963542146","doi":"10.3847/1538-4357/aafac6","title":"A Comprehensive Spectroscopic and Photometric Analysis of DA and DB White Dwarfs from SDSS and Gaia","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; White dwarf; Astrophysics; Photometry (optics); Stars; Parallax; Effective temperature; Spectral line; Spectroscopy; Astronomy; Sky","score_opus":0.009814558798804636,"score_gpt":0.23070480502352225,"score_spread":0.22089024622471762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963542146","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9835212,0.00037047252,0.002022445,0.00003923318,0.000010894992,0.000033526278,0.0107925,0.0002808942,0.0029287522],"genre_scores_gemma":[0.96439916,0.00016472783,0.005110314,0.00006773336,0.000018682074,0.00002500913,0.028863624,0.00009337866,0.0012572504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999658,0.000029685067,0.000028969467,0.000086712076,0.0001364041,0.000060198916],"domain_scores_gemma":[0.99913234,0.000048895305,0.00021227387,0.00013110718,0.00029607007,0.0001793948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005931807,0.0004439667,0.00031422699,0.00453383,0.00054360874,0.00041066724,0.00023161198,0.00011805736,0.0005069555],"category_scores_gemma":[0.0006110973,0.000141937,0.00029053207,0.0021948582,0.00016775525,0.00014067824,0.00045989035,0.00013860824,0.0006725678],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012219041,0.00009033553,0.92447025,0.00007450319,0.00013279401,0.00017586359,0.00039255086,0.001566055,0.03304916,0.00040907844,0.004072027,0.035445195],"study_design_scores_gemma":[0.000004525931,0.00003249974,0.9889775,0.0000074007958,0.000023635028,0.00010645723,0.00011029031,0.0011811848,0.0028764114,0.00009733958,0.0065755,0.0000073319707],"about_ca_topic_score_codex":0.0123648215,"about_ca_topic_score_gemma":0.018517062,"teacher_disagreement_score":0.0123648215,"about_ca_system_score_codex":0.00037705517,"about_ca_system_score_gemma":0.00047735078,"threshold_uncertainty_score":0.024585724},"labels":[],"label_agreement":null},{"id":"W2963645840","doi":"10.1088/0004-637x/788/2/103","title":"WHITE DWARFS IN THE UKIRT INFRARED DEEP SKY SURVEY DATA RELEASE 9","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Physics; Sky; Infrared; Astronomy; Astrophysics; Brown dwarf; Massive compact halo object; Stars; Astrobiology","score_opus":0.023191645221484588,"score_gpt":0.24636846105607077,"score_spread":0.22317681583458618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963645840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90533495,0.02577109,0.0036760892,0.0005737366,0.00020087224,0.00010505903,0.03977575,0.00036475895,0.024197761],"genre_scores_gemma":[0.9164247,0.0077866553,0.003155363,0.00038824585,0.00009641038,0.00006912266,0.06577656,0.000092682654,0.006210169],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955887,0.000027458807,0.0000607432,0.00010185813,0.00015054258,0.00010050732],"domain_scores_gemma":[0.99952805,0.000039834376,0.00021707089,0.00003930468,0.00012008858,0.000055623295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000482175,0.00019966553,0.00021760707,0.001266047,0.0002552925,0.0005449335,0.00035150727,0.00013811099,0.0010888387],"category_scores_gemma":[0.0006668783,0.000088486755,0.00022380652,0.0017193846,0.00014430266,0.00027973746,0.0005004613,0.0001446941,0.00078155706],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019024157,0.000032465556,0.87026554,0.001017014,0.00013206787,0.0009061185,0.0011881824,0.00039656556,0.0102792345,0.0018079707,0.027713103,0.08607149],"study_design_scores_gemma":[0.000007253343,0.000026361457,0.8887369,0.00016501009,0.000059511585,0.00075599557,0.0003398212,0.00015214058,0.0012049305,0.00028695012,0.10825262,0.000012496144],"about_ca_topic_score_codex":0.019248337,"about_ca_topic_score_gemma":0.028065532,"teacher_disagreement_score":0.019248337,"about_ca_system_score_codex":0.00047341935,"about_ca_system_score_gemma":0.00039598398,"threshold_uncertainty_score":0.03827262},"labels":[],"label_agreement":null},{"id":"W2963730462","doi":"10.1088/0004-637x/806/2/266","title":"GREEN BANK TELESCOPE AND<i>SWIFT</i>X-RAY TELESCOPE OBSERVATIONS OF THE GALACTIC CENTER RADIO MAGNETAR SGR J1745–2900","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Magnetar; Physics; Astrophysics; Pulsar; Green Bank Telescope; Radio telescope; Astronomy; Telescope; Flux (metallurgy); Galactic Center; Neutron star; Rotation period; Galaxy; Stars","score_opus":0.026210512921672008,"score_gpt":0.2844506068751129,"score_spread":0.25824009395344094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963730462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99633116,0.00021783712,0.00030729803,0.000035806017,0.000017676783,0.000013167676,0.0018052204,0.00004911566,0.0012227553],"genre_scores_gemma":[0.99002576,0.00015061777,0.0017279375,0.000071893235,0.000054942077,0.000023343031,0.007093176,0.000034904162,0.0008173848],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972564,0.000030444055,0.000017545184,0.00007505513,0.0000842417,0.00006708691],"domain_scores_gemma":[0.999005,0.00007177523,0.00048657996,0.000082521205,0.00009297914,0.0002611101],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004664831,0.0003327809,0.00028654386,0.0020116253,0.0005068173,0.0004252787,0.00035873338,0.00033190078,0.0010361469],"category_scores_gemma":[0.0005946389,0.00023238242,0.00033903553,0.00080021546,0.0002888184,0.0003137268,0.0007622499,0.00030125098,0.00047101022],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000525724,0.00016433967,0.9396195,0.0000803686,0.00026953773,0.00089064805,0.00050563953,0.0011380818,0.039913874,0.00016626544,0.0025625492,0.014163372],"study_design_scores_gemma":[0.000008251099,0.000048869613,0.99786586,0.000003556783,0.000015425054,0.00015865968,0.000049123108,0.00024065253,0.0006239034,0.00001573443,0.0009637831,0.0000062614877],"about_ca_topic_score_codex":0.009494812,"about_ca_topic_score_gemma":0.024023352,"teacher_disagreement_score":0.009494812,"about_ca_system_score_codex":0.00037807954,"about_ca_system_score_gemma":0.00021206828,"threshold_uncertainty_score":0.018879116},"labels":[],"label_agreement":null},{"id":"W2963770711","doi":"10.1088/0004-637x/808/2/160","title":"PHYSICAL PROPERTIES OF A PILOT SAMPLE OF SPECTROSCOPIC CLOSE PAIR GALAXIES AT<i>z</i>∼ 2","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; David and Lucile Packard Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Star formation; Astronomy; Stellar mass; Advanced Camera for Surveys; Spectroscopy; Flux (metallurgy); Line-of-sight; Limiting magnitude; Population","score_opus":0.020723201080604017,"score_gpt":0.22617137314627098,"score_spread":0.20544817206566696,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963770711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995351,0.000011663362,0.00012610493,0.0000050816993,5.8079974e-7,0.00002171976,0.0001166675,0.000009133635,0.00017408059],"genre_scores_gemma":[0.9978562,0.00001923127,0.00057725457,0.000020926254,0.0000069084635,0.00003480683,0.0012029189,0.000004971212,0.00027683377],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979717,0.00003170158,0.000017558692,0.000060818667,0.00004333551,0.00004938227],"domain_scores_gemma":[0.9989674,0.00015954532,0.000206872,0.00019453761,0.00015090444,0.000320816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040823105,0.0003199583,0.00033019017,0.00120058,0.0007705501,0.00041736092,0.00040841612,0.00034659394,0.0016455443],"category_scores_gemma":[0.00096014026,0.00021108362,0.00024939037,0.00057676947,0.00033518646,0.00033602686,0.00067133544,0.00022828803,0.00058484054],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006246924,0.0010697868,0.9535745,0.000027559463,0.000042822623,0.0007139493,0.0014019401,0.00025195148,0.03218878,0.00017616949,0.0004998588,0.009428074],"study_design_scores_gemma":[0.000037613303,0.0006058857,0.9929929,0.0000024235935,0.00002389256,0.0013391244,0.00035582858,0.0006511379,0.003108899,0.000045310808,0.0008302436,0.0000067395085],"about_ca_topic_score_codex":0.0023612664,"about_ca_topic_score_gemma":0.002945527,"teacher_disagreement_score":0.0023612664,"about_ca_system_score_codex":0.00015492164,"about_ca_system_score_gemma":0.00011282674,"threshold_uncertainty_score":0.0055048466},"labels":[],"label_agreement":null},{"id":"W2963812191","doi":"10.3847/1538-4357/ab7ea7","title":"Impact of the Collision Model on the Multi-messenger Emission from Gamma-Ray Burst Internal Shocks","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Collision; Kinetic energy; Cosmic ray; Shock wave; Merge (version control); Plasma; Inelastic collision; Internal energy","score_opus":0.022964455838046825,"score_gpt":0.26106133051546054,"score_spread":0.23809687467741372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963812191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9827399,0.0002935136,0.0076248012,0.00015722687,0.0000447985,0.000021247277,0.00017514118,0.000089308116,0.008854034],"genre_scores_gemma":[0.9987704,0.00008411145,0.00038044478,0.00001887453,0.0000069417238,0.000007573158,0.000060974926,0.000023799237,0.00064701797],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997775,0.0000610264,0.000006729849,0.000033098255,0.000038816568,0.00008280378],"domain_scores_gemma":[0.99938965,0.0003329275,0.00009909239,0.000036780984,0.000058021655,0.00008354274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004645375,0.00063144416,0.0005859829,0.0004492831,0.0005401851,0.0014521705,0.000720288,0.0005360914,0.0034307565],"category_scores_gemma":[0.0014118575,0.00020828108,0.000649588,0.00031157176,0.0005133296,0.00058702636,0.0009164093,0.00043426605,0.00018335573],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050128286,0.00014479399,0.02598403,0.0001317698,0.00014485588,0.0014958762,0.000125625,0.92311996,0.019303482,0.024259992,0.0006223796,0.004166032],"study_design_scores_gemma":[0.00006561243,0.0001183694,0.0064181495,0.000013020602,0.00006279732,0.00018985297,0.00009559134,0.9847097,0.005122815,0.0027210517,0.00045793178,0.000025163848],"about_ca_topic_score_codex":0.0037457496,"about_ca_topic_score_gemma":0.0010948365,"teacher_disagreement_score":0.0037457496,"about_ca_system_score_codex":0.00075619784,"about_ca_system_score_gemma":0.0004635533,"threshold_uncertainty_score":0.011476994},"labels":[],"label_agreement":null},{"id":"W2963893319","doi":"10.1088/0004-637x/807/1/52","title":"A LOW-MASS MAIN-SEQUENCE STAR AND ACCRETION DISK IN THE VERY FAINT X-RAY TRANSIENT M15 X-3","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Accretion (finance); Luminosity; Hubble space telescope; Astronomy; X-ray transient; Accretion disc; Light curve; Neutron star; Stars; Galaxy","score_opus":0.023356825515483064,"score_gpt":0.24258083648117693,"score_spread":0.21922401096569386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963893319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989359,0.0001948079,0.00007440449,0.00006835721,0.000007621533,0.000005837271,0.0000702003,0.0000093508415,0.0006335863],"genre_scores_gemma":[0.9992556,0.000052335847,0.0001252083,0.000050007457,0.000014980206,0.0000037966015,0.00015737324,0.0000067616897,0.00033394803],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999312,0.000005131899,0.000007690546,0.000022222393,0.000014447278,0.00001924608],"domain_scores_gemma":[0.99960154,0.000049259736,0.00016642768,0.000021262938,0.00003181506,0.00012970043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023151396,0.0002957174,0.00047731074,0.00087664725,0.0008531892,0.0007843449,0.0004541739,0.0006798704,0.0010186707],"category_scores_gemma":[0.00045886982,0.0001909848,0.00033491597,0.00060924544,0.0004843786,0.00027441594,0.0009696684,0.00043376134,0.0003308907],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007684557,0.00013199396,0.9420455,0.00006064358,0.000056915178,0.0046498915,0.0007193683,0.00017288538,0.04512663,0.00046132566,0.00044242325,0.005363903],"study_design_scores_gemma":[0.000014169324,0.00008885911,0.99643624,0.000010536719,0.00001790038,0.0016827371,0.00019721927,0.00021912907,0.0008729276,0.000100473015,0.00035572876,0.0000041237636],"about_ca_topic_score_codex":0.0038452642,"about_ca_topic_score_gemma":0.0052871113,"teacher_disagreement_score":0.0038452642,"about_ca_system_score_codex":0.00061617565,"about_ca_system_score_gemma":0.00028623885,"threshold_uncertainty_score":0.007645786},"labels":[],"label_agreement":null},{"id":"W2963959280","doi":"10.3847/1538-4357/aa5c3f","title":"Photoionization Models for the Inner Gaseous Disks of Herbig Be Stars: Evidence against Magnetospheric Accretion?*","year":2017,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Radiative transfer; Emission spectrum; Line (geometry); Spectral line; Photoionization; Stars; Radiative equilibrium; Be star","score_opus":0.03769588031183481,"score_gpt":0.2821302184717542,"score_spread":0.24443433815991938,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2963959280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99570674,0.00007968486,0.0023164342,0.000060957176,0.0000029693408,0.000009141915,0.000081213504,0.0000364539,0.0017063487],"genre_scores_gemma":[0.999302,0.000031160234,0.00037921895,0.000011643885,0.0000027259753,0.0000050402036,0.000045816167,0.000006885529,0.00021554228],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994445,0.000012752158,0.0000030626697,0.00001478777,0.000009298624,0.000015582336],"domain_scores_gemma":[0.9998709,0.000041739284,0.000029374538,0.000015349548,0.000015788915,0.000026915002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017884013,0.00035231566,0.00032019446,0.00037284076,0.0004477796,0.00067712425,0.0008976455,0.0007109346,0.00080784684],"category_scores_gemma":[0.00047988992,0.00020924768,0.00040601226,0.0002349057,0.00034016982,0.0006026806,0.00028854838,0.00017746995,0.00019029355],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020965506,0.00012132064,0.09435838,0.000043445452,0.00009676529,0.0005350468,0.00027434027,0.87762076,0.017528487,0.0037282284,0.00030363776,0.005179942],"study_design_scores_gemma":[0.00006373227,0.00006489656,0.03041905,0.000006098355,0.000021961521,0.000089029796,0.000104691055,0.9659985,0.0014933364,0.0013188744,0.00040651162,0.000013389213],"about_ca_topic_score_codex":0.020963687,"about_ca_topic_score_gemma":0.0067756404,"teacher_disagreement_score":0.020963687,"about_ca_system_score_codex":0.000915339,"about_ca_system_score_gemma":0.00021429746,"threshold_uncertainty_score":0.041683376},"labels":[],"label_agreement":null},{"id":"W2964045908","doi":"10.1088/0004-637x/814/1/71","title":"THE CARINA PROJECT. IX. ON HYDROGEN AND HELIUM BURNING VARIABLES","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"RR Lyrae variable; Physics; Cepheid variable; Astrophysics; Distance modulus; Metallicity; Dwarf spheroidal galaxy; Variable star; Galaxy; Luminosity; Astronomy; Cosmic distance ladder; Red clump; Galactic halo; Milky Way; Population; Halo; Dwarf galaxy; Stars; Globular cluster","score_opus":0.018946847469632787,"score_gpt":0.2382506899225108,"score_spread":0.219303842452878,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964045908","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.030933121,0.0155724995,0.017271569,0.0037664236,0.00091619964,0.00067952485,0.77751535,0.031199668,0.12214557],"genre_scores_gemma":[0.04887528,0.003281718,0.038728427,0.00095694984,0.0005484372,0.001401033,0.8550867,0.009244827,0.041876636],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99854445,0.00035555687,0.00006801795,0.0004130897,0.00038134953,0.0002375659],"domain_scores_gemma":[0.9973188,0.00045411152,0.00036119384,0.0007898756,0.0005195205,0.00055650424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032377432,0.0020183877,0.0010844758,0.004737113,0.00094968476,0.0040207705,0.0021333059,0.001072532,0.04077801],"category_scores_gemma":[0.0042011207,0.00066292577,0.00084086333,0.004878088,0.0004733056,0.0018515844,0.005013739,0.0010501157,0.03955018],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017565315,0.0002090987,0.029714022,0.0015735496,0.0003290067,0.00033155776,0.00086476054,0.0015302021,0.0028112254,0.019186864,0.68016356,0.26152965],"study_design_scores_gemma":[0.00024245857,0.00007113003,0.02691315,0.00040589494,0.00008840186,0.00019862497,0.00022312804,0.00180014,0.0011497599,0.0065164305,0.96234727,0.00004365551],"about_ca_topic_score_codex":0.023299042,"about_ca_topic_score_gemma":0.015896237,"teacher_disagreement_score":0.04077801,"about_ca_system_score_codex":0.0010229523,"about_ca_system_score_gemma":0.0021883203,"threshold_uncertainty_score":0.13641602},"labels":[],"label_agreement":null},{"id":"W2964077033","doi":"10.1088/0004-637x/798/1/49","title":"HYDRODYNAMIC SIMULATIONS OF H ENTRAINMENT AT THE TOP OF He-SHELL FLASH CONVECTION","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":100,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Convection; Mechanics; Entrainment (biomusicology); Convection zone; Astrophysics; Classical mechanics","score_opus":0.006228162194929766,"score_gpt":0.21308171583236343,"score_spread":0.20685355363743366,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964077033","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.993042,0.000065738415,0.0025155148,0.0001363681,0.000018849214,0.000035499284,0.00034128863,0.00010300291,0.0037417456],"genre_scores_gemma":[0.99682605,0.000032451666,0.0020702702,0.000042336662,0.000007339944,0.000031340383,0.00031647476,0.000026042124,0.00064778957],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998652,0.000023176974,0.00000735212,0.000016903194,0.000026586698,0.00006078981],"domain_scores_gemma":[0.99953973,0.00018665097,0.00005701068,0.00003059835,0.000055626704,0.0001304623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026218483,0.0004605879,0.0006969901,0.0003457074,0.0006158973,0.00066745793,0.0008334106,0.0010751069,0.0016571349],"category_scores_gemma":[0.0012014941,0.00026209585,0.0005715534,0.0004757264,0.0010145932,0.00041079687,0.0007246797,0.0008801922,0.00012251151],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029063752,0.0001804847,0.0069363657,0.00003686151,0.000048699625,0.0002820434,0.0001798675,0.9813871,0.006492615,0.0021621834,0.00031465237,0.0016885696],"study_design_scores_gemma":[0.00006850702,0.00006203158,0.0021838718,0.0000043172795,0.0000074091095,0.000015213194,0.00004830093,0.9961443,0.0009326338,0.00036072734,0.00016349643,0.000009275291],"about_ca_topic_score_codex":0.0211409,"about_ca_topic_score_gemma":0.007878134,"teacher_disagreement_score":0.0211409,"about_ca_system_score_codex":0.00094172417,"about_ca_system_score_gemma":0.0009976232,"threshold_uncertainty_score":0.0420357},"labels":[],"label_agreement":null},{"id":"W2964112700","doi":"10.3847/1538-4357/ab5792","title":"The Spectral Evolution of AT 2018dyb and the Presence of Metal Lines in Tidal Disruption Events","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":127,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Science and Technology Facilities Council; Horizon 2020 Framework Programme; Council for Higher Education; United States-Israel Binational Science Foundation; Danmarks Grundforskningsfond; Canadian Institute for Advanced Research; Alexander von Humboldt-Stiftung","keywords":"Physics; Balmer series; Astrophysics; Spectral line; Emission spectrum; Lambda; Accretion (finance); Light curve; Luminosity; Black hole (networking); Astronomy; Optics; Galaxy","score_opus":0.0073480059929537525,"score_gpt":0.22935704547228447,"score_spread":0.2220090394793307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964112700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99723095,0.000045300814,0.00009533236,0.000032022854,0.0000047938975,0.0000038936223,0.0009851649,0.000027663433,0.0015748537],"genre_scores_gemma":[0.9975926,0.000026661322,0.00014666357,0.000010442019,0.000007739333,0.000006311084,0.0016376007,0.0000096272925,0.00056228065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991226,0.000006720589,0.0000045968895,0.000020666039,0.000029536322,0.000026146927],"domain_scores_gemma":[0.99945384,0.000051057905,0.00018436559,0.000025160201,0.00009936288,0.00018626491],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013312645,0.00017617743,0.00019583371,0.0015668992,0.00028457193,0.00047567723,0.00018263982,0.0002336158,0.0021442121],"category_scores_gemma":[0.00049515493,0.00008495318,0.00014207268,0.0009316399,0.00019279691,0.0002100823,0.00043393273,0.00020253129,0.00060977845],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029003358,0.00007667351,0.9692183,0.000028684562,0.000023744782,0.0003288148,0.00033766474,0.00047270933,0.016301936,0.00015834572,0.0011114965,0.011651657],"study_design_scores_gemma":[0.0000021662117,0.000020082649,0.99825674,0.000002608384,0.0000026895639,0.000073640935,0.00008090436,0.00024869916,0.00047212347,0.000023986344,0.0008136693,0.0000027063913],"about_ca_topic_score_codex":0.0052610966,"about_ca_topic_score_gemma":0.0072242464,"teacher_disagreement_score":0.0052610966,"about_ca_system_score_codex":0.0004205387,"about_ca_system_score_gemma":0.00007259746,"threshold_uncertainty_score":0.010460913},"labels":[],"label_agreement":null},{"id":"W2964332121","doi":"10.1088/0004-637x/807/1/44","title":"SPACING OF<i>KEPLER</i>PLANETS: SCULPTING BY DYNAMICAL INSTABILITY","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":267,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Planet; Transit (satellite); Planetary system; Astronomy; Instability; Astrophysics; Kepler; Astrobiology; Mechanics","score_opus":0.014337640809646321,"score_gpt":0.23023183957405047,"score_spread":0.21589419876440413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964332121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99901223,0.000018304585,0.0005168372,0.000027009144,0.0000010915838,0.0000013359451,0.000023188362,0.000010450876,0.00038951813],"genre_scores_gemma":[0.9996847,0.000008475142,0.00021559623,0.0000035650917,7.675855e-7,0.0000013334077,0.000034611887,0.0000044683397,0.00004652003],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992955,0.0000140842685,0.000003862933,0.00002377397,0.0000102824,0.000018504066],"domain_scores_gemma":[0.9992244,0.00022049966,0.00028187223,0.000061347855,0.0000591712,0.00015274744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030380412,0.00017863935,0.00021126766,0.0004659829,0.00042869424,0.0005363991,0.00034912443,0.00030831483,0.00073865906],"category_scores_gemma":[0.0019770223,0.00018570127,0.0003152412,0.00032680322,0.0005808809,0.00054414687,0.0005146808,0.00033170433,0.00009859626],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043687518,0.00012991315,0.5140158,0.00005933433,0.00021365951,0.00060911226,0.0005206077,0.44595382,0.023524804,0.0060386485,0.0008121043,0.007685437],"study_design_scores_gemma":[0.000046554804,0.00012540068,0.13676809,0.000009556448,0.000039104943,0.0002316528,0.00023723699,0.8558707,0.002774104,0.003429843,0.00044350835,0.000024361529],"about_ca_topic_score_codex":0.005412745,"about_ca_topic_score_gemma":0.0043374556,"teacher_disagreement_score":0.005412745,"about_ca_system_score_codex":0.0006113948,"about_ca_system_score_gemma":0.00027157762,"threshold_uncertainty_score":0.010762513},"labels":[],"label_agreement":null},{"id":"W2964622611","doi":"10.3847/1538-4357/ab3403","title":"An Exo–Kuiper Belt with an Extended Halo around HD 191089 in Scattered Light","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Western University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; California Institute of Technology; National Aeronautics and Space Administration; Ministerio de Ciencia, Tecnología e Innovación Productiva; Maryland Advanced Research Computing Center; Jet Propulsion Laboratory; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Halo; Astronomy; Physics; Astrobiology; Astrophysics","score_opus":0.008097169685389644,"score_gpt":0.22513692306446673,"score_spread":0.21703975337907708,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2964622611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99930215,0.000032609714,0.00021041156,0.000013295973,0.000002169285,0.00000356508,0.00008405069,0.000022481152,0.00032928772],"genre_scores_gemma":[0.99957496,0.0000097298725,0.00020176219,0.0000051162338,0.0000028532047,0.0000017185386,0.00014393711,0.0000038446933,0.00005617254],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992096,0.00001781405,0.0000053076146,0.000021449643,0.000016619002,0.000017866181],"domain_scores_gemma":[0.9997212,0.000045976267,0.00007351682,0.000060109902,0.000033855315,0.000065278306],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040176322,0.00027563656,0.00025827813,0.00064639485,0.00045457523,0.0005230074,0.0006692073,0.000281313,0.0009839681],"category_scores_gemma":[0.0005815005,0.00024944745,0.00041608734,0.0005048126,0.00028393208,0.00021277858,0.0006242486,0.00018137867,0.0002327241],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008665877,0.00022361924,0.9233168,0.000045286954,0.00025671688,0.002750216,0.0005982296,0.019330988,0.04397416,0.0005606656,0.0005210626,0.0075557316],"study_design_scores_gemma":[0.000069183036,0.00013927658,0.9696471,0.0000148972695,0.00005478458,0.00059833855,0.0002769716,0.026187448,0.0018645374,0.00022068986,0.00090952055,0.000017308943],"about_ca_topic_score_codex":0.010040323,"about_ca_topic_score_gemma":0.008865986,"teacher_disagreement_score":0.010040323,"about_ca_system_score_codex":0.0005151508,"about_ca_system_score_gemma":0.00014327394,"threshold_uncertainty_score":0.019963741},"labels":[],"label_agreement":null},{"id":"W2965189278","doi":"10.3847/1538-4357/ab3a9b","title":"A Triple AGN in a Mid-infrared Selected Late-stage Galaxy Merger","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Supermassive black hole; Active galactic nucleus; Galaxy; Galaxy merger; Star formation; Accretion (finance); Galaxy formation and evolution; Emission spectrum","score_opus":0.006086627710530072,"score_gpt":0.20605348928955047,"score_spread":0.1999668615790204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2965189278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998154,0.00006570344,0.00062217785,0.00016701159,0.000010223794,0.000010068821,0.000029520821,0.000018487457,0.0009227637],"genre_scores_gemma":[0.99951696,0.000009105942,0.00026109375,0.000044346478,0.000009662639,0.0000014196543,0.000024956506,0.0000017715445,0.00013073043],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999876,0.0000125690485,0.00000818358,0.000033067157,0.000024290935,0.000045730438],"domain_scores_gemma":[0.9997049,0.00003517962,0.0000704926,0.000020351375,0.000020696441,0.0001482508],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020390798,0.00018931391,0.0002635482,0.0006903737,0.00100119,0.0007308926,0.0003667822,0.0008976413,0.0011712617],"category_scores_gemma":[0.00053168676,0.00015429393,0.00021149903,0.00025436803,0.0004068718,0.00030170914,0.00087123696,0.00060155377,0.0002068086],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010978361,0.00058623526,0.5682747,0.0000477452,0.00011159963,0.31339005,0.0015941508,0.0019165373,0.08827048,0.0045384406,0.0014929972,0.018679345],"study_design_scores_gemma":[0.00011658177,0.0012999802,0.6494958,0.000025085128,0.00009677032,0.30647144,0.0020201933,0.017685646,0.014140857,0.0037518514,0.00482623,0.00006956982],"about_ca_topic_score_codex":0.0015366502,"about_ca_topic_score_gemma":0.002234422,"teacher_disagreement_score":0.0015366502,"about_ca_system_score_codex":0.00043052304,"about_ca_system_score_gemma":0.0001228326,"threshold_uncertainty_score":0.0039182305},"labels":[],"label_agreement":null},{"id":"W2965488712","doi":"10.3847/1538-4357/ab7b7b","title":"Variability of Massive Stars in M31 from the Palomar Transient Factory","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Gordon and Betty Moore Foundation","keywords":"Stars; Supergiant; Astrophysics; Physics; Light curve; Hertzsprung–Russell diagram; Variable star; Amplitude; Observatory; Astronomy; Stellar evolution","score_opus":0.014240606151311577,"score_gpt":0.2116397829378142,"score_spread":0.19739917678650265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2965488712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983767,0.00003062177,0.00023819426,0.000012371523,0.0000011773773,0.0000053701306,0.0009916148,0.000030831612,0.00031310582],"genre_scores_gemma":[0.9964954,0.000013770012,0.0002328779,0.000006086932,0.0000039246024,0.000008086185,0.0031304855,0.00000811001,0.0001013368],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975723,0.000036486388,0.000013832171,0.00007861684,0.000056041135,0.00005779471],"domain_scores_gemma":[0.9984396,0.00024363345,0.0006079697,0.00021704097,0.00017055281,0.00032113522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053910416,0.0002372036,0.0002991297,0.0016321323,0.00027357478,0.0005996573,0.0002754621,0.00021567308,0.0011632362],"category_scores_gemma":[0.0014626127,0.00010519839,0.00028759564,0.001437509,0.00021200922,0.00027526074,0.0006854871,0.0002074552,0.0006087657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011228019,0.000022206845,0.98953605,0.000010517047,0.000028139923,0.00016037721,0.00019273476,0.0005104191,0.0037633374,0.00006581258,0.00042888522,0.0051692477],"study_design_scores_gemma":[0.0000027750862,0.000017485041,0.998917,0.0000016175948,0.000002715995,0.0000593214,0.00004055891,0.0004913358,0.000177319,0.000017565499,0.00027027246,0.0000019771028],"about_ca_topic_score_codex":0.0064228023,"about_ca_topic_score_gemma":0.0059948605,"teacher_disagreement_score":0.0064228023,"about_ca_system_score_codex":0.00041119102,"about_ca_system_score_gemma":0.000174711,"threshold_uncertainty_score":0.012770832},"labels":[],"label_agreement":null},{"id":"W2965524853","doi":"10.3847/1538-4357/ab2885","title":"Testing Seismic Models of Hot B Subdwarfs with Gaia Data","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National d’Etudes Spatiales; Fonds De La Recherche Scientifique - FNRS; National Aeronautics and Space Administration; Agence Nationale de la Recherche; European Space Agency; California Institute of Technology; Jet Propulsion Laboratory; Université de Montréal; Deutsche Forschungsgemeinschaft","keywords":"Physics; Parallax; Photometry (optics); Astrophysics; Stars; Astronomy; Extinction (optical mineralogy); Surface gravity; Optics","score_opus":0.03197987446811352,"score_gpt":0.2330991395218277,"score_spread":0.2011192650537142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2965524853","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967056,0.00003251894,0.002083455,0.0000739646,0.0000052459877,0.00001643983,0.0002553318,0.00008407392,0.00074348715],"genre_scores_gemma":[0.99861753,0.000017248234,0.00073495146,0.0000144052,0.0000042467127,0.000008227851,0.0005136852,0.00001841055,0.00007124066],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99909055,0.00035758165,0.00006129396,0.00024213211,0.0001386248,0.00010974713],"domain_scores_gemma":[0.99292094,0.0042275502,0.0010665959,0.00073089526,0.00057628594,0.0004777189],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0041685514,0.000609686,0.0005380453,0.0012632103,0.0004569403,0.0017112283,0.0017318734,0.00062218757,0.001093732],"category_scores_gemma":[0.008834962,0.00035551318,0.0008890502,0.001000561,0.0007247947,0.0010707593,0.0010792742,0.0005469898,0.00032288162],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009281104,0.00017677435,0.6367387,0.00005358114,0.00039285776,0.0002666258,0.0006937811,0.34316546,0.003397849,0.0034091233,0.0006076283,0.010169549],"study_design_scores_gemma":[0.00011540345,0.0002595439,0.117095076,0.000022016544,0.00007880436,0.00007516367,0.00056888553,0.8777709,0.001536977,0.001512458,0.0009270532,0.000037706533],"about_ca_topic_score_codex":0.020572219,"about_ca_topic_score_gemma":0.0067105344,"teacher_disagreement_score":0.020572219,"about_ca_system_score_codex":0.0021789032,"about_ca_system_score_gemma":0.00086865167,"threshold_uncertainty_score":0.04090494},"labels":[],"label_agreement":null},{"id":"W2965895666","doi":"10.3847/1538-4357/ab4a7f","title":"Chandra Spectral and Timing Analysis of Sgr A*'s Brightest X-Ray Flares","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; McGill University; Canadian Institute for Advanced Research","funders":"Natural Sciences and Engineering Research Council of Canada; Fonds de recherche du Québec – Nature et technologies; Max-Planck-Gesellschaft; Canadian Institute for Advanced Research; Bundesministerium für Wirtschaft und Technologie; McGill University; National Aeronautics and Space Administration; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Smithsonian Institution","keywords":"Flare; Accretion (finance); Static timing analysis; Spectral index; Flare star; Spectral density; Accretion disc; Luminosity; Spectral line","score_opus":0.010533140850350979,"score_gpt":0.2261667748240917,"score_spread":0.21563363397374072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2965895666","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961582,0.0001305557,0.0004885401,0.000030136598,0.00001148228,0.000011553205,0.0013823395,0.00016777679,0.0016194388],"genre_scores_gemma":[0.995365,0.000049712336,0.0013016295,0.000026231359,0.000018178736,0.000009868218,0.0028555566,0.000030860265,0.00034298337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982184,0.000009838397,0.000013203279,0.000043534917,0.000051593637,0.000060027327],"domain_scores_gemma":[0.99885535,0.00015097503,0.00039974577,0.0001098747,0.00018711002,0.00029705974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024635566,0.0002560206,0.0002951214,0.0039497754,0.0004512115,0.0007214184,0.00029320226,0.00025575492,0.0012211732],"category_scores_gemma":[0.00078723487,0.00012857164,0.00052162184,0.0013756485,0.00015740369,0.00021488588,0.00037120137,0.0002891333,0.00028079934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010281882,0.0003222863,0.8505415,0.00015209432,0.0004356925,0.0010976847,0.0003337475,0.0044518257,0.09011644,0.0012479818,0.0034567025,0.046815973],"study_design_scores_gemma":[0.0000085760585,0.000053970194,0.9931716,0.000005755887,0.000030186548,0.00035954267,0.00006115665,0.0026482448,0.0023022045,0.00007558914,0.0012674606,0.000015776179],"about_ca_topic_score_codex":0.007287111,"about_ca_topic_score_gemma":0.007970934,"teacher_disagreement_score":0.007287111,"about_ca_system_score_codex":0.00029722106,"about_ca_system_score_gemma":0.0003167665,"threshold_uncertainty_score":0.014489412},"labels":[],"label_agreement":null},{"id":"W2965935603","doi":"10.3847/1538-4357/ab371a","title":"The Filamentary Radio Lobes of the Seyfert–Starburst Composite Galaxy NGC 3079","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Faraday effect; Radio galaxy; Magnetic field; X-shaped radio galaxy; Polarization (electrochemistry); Galaxy; Population; Dynamo; Linear polarization","score_opus":0.004104828757745605,"score_gpt":0.18969524062312054,"score_spread":0.18559041186537495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2965935603","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990375,0.0000467785,0.000109124,0.000011001494,0.000001551191,0.0000012906304,0.00024696998,0.0000114627555,0.00053441554],"genre_scores_gemma":[0.99948287,0.000020155137,0.00011603007,0.0000039731935,0.0000026989069,0.0000013414576,0.0002970279,0.0000019474176,0.00007392628],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994373,0.0000067844576,0.0000040596938,0.000018116647,0.000011521046,0.000015797883],"domain_scores_gemma":[0.99963176,0.000059203845,0.00015317534,0.00004493831,0.000028578124,0.000082377046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011987066,0.00014594925,0.00017805879,0.00070621644,0.0002749725,0.00036430394,0.00017183644,0.00012687476,0.0014587006],"category_scores_gemma":[0.00022877502,0.00011229309,0.00018891649,0.00037208552,0.00022354678,0.00016563051,0.0002931964,0.0001409621,0.00020584915],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066519657,0.00005902047,0.86029875,0.000059002123,0.00012793057,0.0012264628,0.0004560699,0.0015962807,0.12543409,0.000393741,0.00065695326,0.0090264985],"study_design_scores_gemma":[0.000005261967,0.000027899188,0.9971591,0.0000049748755,0.0000126888235,0.00029999146,0.00009052537,0.00060801045,0.0014014901,0.000092359696,0.00029371143,0.0000039168335],"about_ca_topic_score_codex":0.0032890064,"about_ca_topic_score_gemma":0.00498392,"teacher_disagreement_score":0.0032890064,"about_ca_system_score_codex":0.00021791956,"about_ca_system_score_gemma":0.00007405774,"threshold_uncertainty_score":0.006539762},"labels":[],"label_agreement":null},{"id":"W2966443322","doi":"10.3847/1538-4357/ab379e","title":"A Photometric and Spectroscopic Investigation of the DB White Dwarf Population Using SDSS and Gaia Data","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Photometry (optics); Sky; Parallax; Population; Spectroscopy; Stellar population; Stars","score_opus":0.023990541331946825,"score_gpt":0.25024558334414887,"score_spread":0.22625504201220203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2966443322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959045,0.00012586649,0.0005970635,0.000014626068,0.0000021635883,0.0000111261625,0.002120154,0.000036123514,0.0011885321],"genre_scores_gemma":[0.9933897,0.00007947472,0.0009247553,0.000011982444,0.000007647628,0.000007563405,0.005224688,0.000013709618,0.00034034465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973565,0.00003468188,0.000020381292,0.00007171567,0.000084720225,0.000052838084],"domain_scores_gemma":[0.99931383,0.00006966321,0.00017198191,0.000097123,0.00017856738,0.00016875846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005520807,0.00026729773,0.00023932743,0.003931986,0.00042401775,0.00045344108,0.00022642917,0.00009784575,0.0006158888],"category_scores_gemma":[0.00061959826,0.00010929524,0.00021687674,0.0023739699,0.00021245706,0.00019839671,0.00054976204,0.00012070557,0.00036686208],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000069411675,0.000039141192,0.9791326,0.000021819911,0.00005665357,0.00008805609,0.00030348613,0.0006058709,0.006634493,0.00033188,0.00057717186,0.012139452],"study_design_scores_gemma":[0.0000024344583,0.000020853442,0.9970868,0.000002367578,0.0000103752955,0.00006217559,0.00014004699,0.0007713678,0.0006213478,0.00005406532,0.001225452,0.000002708985],"about_ca_topic_score_codex":0.014772313,"about_ca_topic_score_gemma":0.021529095,"teacher_disagreement_score":0.014772313,"about_ca_system_score_codex":0.000351984,"about_ca_system_score_gemma":0.00029425998,"threshold_uncertainty_score":0.029372692},"labels":[],"label_agreement":null},{"id":"W2966584598","doi":"10.1088/0004-637x/780/1/41","title":"THE GAS-RICH CIRCUMBINARY DISK OF HR 4049. I. A DETAILED STUDY OF THE MID-INFRARED SPECTRUM","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Infrared; Circumbinary planet; Astrophysics; Physics; Astronomy; Infrared excess; Wavelength; Spectrometer; Stars; Optics","score_opus":0.007965378342298273,"score_gpt":0.22039971591881136,"score_spread":0.2124343375765131,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2966584598","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966354,0.0004198645,0.00015102873,0.00001351552,0.0000024673047,0.0000041970147,0.00033011186,0.000018781808,0.0024245875],"genre_scores_gemma":[0.99817383,0.00013295452,0.00025179182,0.000019429104,0.000005662707,0.000004817409,0.0008398157,0.000009332594,0.00056217646],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999964,0.0000024407314,0.0000015370526,0.000013164906,0.0000074046243,0.000011465728],"domain_scores_gemma":[0.9999597,0.0000053009053,0.000013755483,0.000004636036,0.0000036562942,0.000012961798],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000047159974,0.00023843734,0.0001642722,0.0005948838,0.00029531532,0.00027769478,0.00027759047,0.0002550582,0.0018591603],"category_scores_gemma":[0.00007704355,0.00009117687,0.00014004117,0.0003815401,0.00016291418,0.00020125769,0.0003351996,0.00011671205,0.00040260036],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081286347,0.00016201317,0.36491778,0.00022030764,0.000113632,0.0043979143,0.00062906917,0.004705361,0.5932482,0.0014434376,0.001174242,0.028175218],"study_design_scores_gemma":[0.000008847622,0.00006679857,0.9939131,0.000008851968,0.000015264799,0.0004936222,0.000083655475,0.0015304235,0.002047721,0.00018693255,0.0016395272,0.000005254245],"about_ca_topic_score_codex":0.002815977,"about_ca_topic_score_gemma":0.0032744794,"teacher_disagreement_score":0.002815977,"about_ca_system_score_codex":0.00031982714,"about_ca_system_score_gemma":0.000050351733,"threshold_uncertainty_score":0.0062195063},"labels":[],"label_agreement":null},{"id":"W2966588803","doi":"10.3847/1538-4357/ab3725","title":"The Next Generation Fornax Survey (NGFS). VI. The Alignment of Dwarf Galaxies in the Fornax Cluster","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Natural Science Foundation of China","keywords":"Fornax Cluster; Galaxy; Dwarf galaxy; Cluster (spacecraft); SIGNAL (programming language); Stars; Dwarf spheroidal galaxy; Brown dwarf","score_opus":0.02077866428891316,"score_gpt":0.2301605067745136,"score_spread":0.20938184248560043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2966588803","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98727334,0.00034578587,0.00022555242,0.00011176126,0.00001465195,0.000014869135,0.007264082,0.00009854192,0.00465154],"genre_scores_gemma":[0.9865645,0.00007135007,0.0010612642,0.000035734094,0.000020169593,0.00001467372,0.010061694,0.000022966226,0.0021476625],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974185,0.000036466172,0.000010357217,0.00008939297,0.0000642209,0.000057647783],"domain_scores_gemma":[0.99929726,0.000050789913,0.00026467716,0.0000915006,0.000117741925,0.00017806787],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005543895,0.00017288663,0.00020537159,0.0010609708,0.00038785694,0.00033357184,0.00025057062,0.00021601883,0.0016098883],"category_scores_gemma":[0.0008995,0.000082668754,0.00020783236,0.0006299819,0.00015313104,0.00027576718,0.00064153987,0.00017448392,0.0005932805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015713234,0.00001826462,0.97564405,0.00004069533,0.00006130103,0.000066277404,0.0002517307,0.00026828583,0.004540048,0.000330063,0.003915444,0.014706691],"study_design_scores_gemma":[0.000002808516,0.000011111467,0.9978916,0.0000033454912,0.000007389398,0.000024046132,0.00004340556,0.00014900847,0.00017291978,0.00002998134,0.0016622025,0.0000021829483],"about_ca_topic_score_codex":0.038418107,"about_ca_topic_score_gemma":0.05807975,"teacher_disagreement_score":0.038418107,"about_ca_system_score_codex":0.00060097786,"about_ca_system_score_gemma":0.00034469194,"threshold_uncertainty_score":0.076389015},"labels":[],"label_agreement":null},{"id":"W2966699747","doi":"10.3847/1538-4357/ab9013","title":"Polarization of the Cosmic Infrared Background Fluctuations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Cosmic infrared background; Cosmic microwave background; Polarization (electrochemistry); Cosmic background radiation; Infrared; COSMIC cancer database; Linear polarization; Galaxy","score_opus":0.012472043058540128,"score_gpt":0.2415206868271791,"score_spread":0.22904864376863895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2966699747","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9411884,0.00019470857,0.032824297,0.00020123097,0.00003385054,0.000012494708,0.0009891295,0.00038184706,0.024173973],"genre_scores_gemma":[0.99874926,0.00004166496,0.0005187259,0.000012996827,0.00000894954,0.0000029938806,0.00026788109,0.000019141376,0.00037833696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998006,0.00004716134,0.0000035161336,0.00005963833,0.000050168903,0.000038862105],"domain_scores_gemma":[0.9995524,0.00013773209,0.00007673663,0.000060192102,0.00011782862,0.000055060766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030166976,0.0003232161,0.00013517877,0.0006839588,0.00014879862,0.00070852734,0.0001751679,0.00016059159,0.0021840741],"category_scores_gemma":[0.001832253,0.00013068678,0.00013475072,0.0005930439,0.00037749158,0.00034110103,0.0002473017,0.0002815604,0.00034763367],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076633325,0.00014452913,0.45129237,0.00015179896,0.00024454002,0.000658736,0.00018421568,0.21838337,0.097834304,0.15113424,0.0070345434,0.07217112],"study_design_scores_gemma":[0.00003913714,0.00010017092,0.36665612,0.000032564247,0.000038135742,0.0003240571,0.000080942526,0.56727296,0.024176558,0.038072452,0.003148968,0.000057833444],"about_ca_topic_score_codex":0.0014302616,"about_ca_topic_score_gemma":0.00062311924,"teacher_disagreement_score":0.0021840741,"about_ca_system_score_codex":0.0003593541,"about_ca_system_score_gemma":0.00016208862,"threshold_uncertainty_score":0.007306397},"labels":[],"label_agreement":null},{"id":"W2967211577","doi":"10.1086/321385","title":"Self‐similar Hot Accretion Flow onto a Neutron Star","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Angular momentum; Accretion (finance); Neutron star; Astrophysics; Angular velocity; RADIUS; Schwarzschild metric; Mechanics; Classical mechanics","score_opus":0.01271671756792121,"score_gpt":0.22893683027847625,"score_spread":0.21622011271055505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2967211577","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9502529,0.0001935759,0.027914623,0.00034593485,0.00010085488,0.00005980437,0.00010413458,0.00015126241,0.02087694],"genre_scores_gemma":[0.9909044,0.00006983047,0.004829399,0.00008797019,0.00003848216,0.00002914084,0.0000728948,0.000023324612,0.0039446037],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998951,0.000030139392,0.000005518193,0.000015581983,0.000023733985,0.000029936517],"domain_scores_gemma":[0.99967706,0.000091834416,0.00008163016,0.000026024041,0.000059846538,0.00006362804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034367235,0.0003949909,0.0005381674,0.0005369963,0.00072619406,0.00088723877,0.00059537217,0.0012930774,0.0016687798],"category_scores_gemma":[0.0017537879,0.0002876088,0.0006317598,0.00029220516,0.0011984834,0.00062102365,0.0007081986,0.0004113396,0.00016619368],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013462156,0.000103110484,0.003935064,0.0000739075,0.000051786625,0.00072503195,0.00022684687,0.954905,0.006596089,0.029982165,0.00063399284,0.002632529],"study_design_scores_gemma":[0.000047215646,0.000031284457,0.0010766236,0.000008194934,0.0000072127864,0.00006929272,0.000043301203,0.9951061,0.00055605546,0.0026224924,0.00042316146,0.000009089722],"about_ca_topic_score_codex":0.005267329,"about_ca_topic_score_gemma":0.0019953107,"teacher_disagreement_score":0.005267329,"about_ca_system_score_codex":0.001104967,"about_ca_system_score_gemma":0.00059970416,"threshold_uncertainty_score":0.010473311},"labels":[],"label_agreement":null},{"id":"W2968035542","doi":"10.3847/1538-4357/ab39dd","title":"Magnetic Fields in the Infrared Dark Cloud G34.43+0.24","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Victoria; McMaster University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Magnetic field; James Clerk Maxwell Telescope; Field (mathematics); Field strength; Magnetohydrodynamics; Velocity dispersion; Infrared; Perpendicular","score_opus":0.007556962992339246,"score_gpt":0.22210059084766112,"score_spread":0.21454362785532188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2968035542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985719,0.000048879854,0.00006972843,0.00002845424,0.0000026137175,0.000004934327,0.00028049873,0.000040177954,0.0009527942],"genre_scores_gemma":[0.999255,0.000018125522,0.00019127311,0.000020278918,0.000004939511,0.0000032702928,0.0003985813,0.000009688237,0.0000989076],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999187,0.000005805921,0.0000019947006,0.0000207239,0.000017164995,0.00003551609],"domain_scores_gemma":[0.99984586,0.000008294495,0.000038272316,0.000013177845,0.000023706509,0.00007062879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010034034,0.00032530897,0.00029401714,0.0008034257,0.00060708396,0.0003943915,0.00035866446,0.00026497807,0.0011439077],"category_scores_gemma":[0.00024940915,0.0001854272,0.00015047856,0.0006205338,0.00025163192,0.00012523955,0.00049687707,0.00037082186,0.00027210635],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009278447,0.00022961157,0.78041965,0.00006194055,0.00011666127,0.001709259,0.0007592963,0.005163047,0.18839514,0.00097140664,0.0024232892,0.01882277],"study_design_scores_gemma":[0.00002792468,0.000042669562,0.99612844,0.0000047998456,0.000013647496,0.000092617745,0.000083251936,0.0014367979,0.0010194028,0.00007666164,0.0010665245,0.0000072865887],"about_ca_topic_score_codex":0.019197462,"about_ca_topic_score_gemma":0.020566668,"teacher_disagreement_score":0.019197462,"about_ca_system_score_codex":0.0006634437,"about_ca_system_score_gemma":0.00020616481,"threshold_uncertainty_score":0.03817147},"labels":[],"label_agreement":null},{"id":"W2968122134","doi":"10.3847/1538-4357/ab3798","title":"The Distribution of Dense Cores near H ii Regions","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Stars; Cluster (spacecraft); Mass distribution; Core (optical fiber); Star cluster; Volume (thermodynamics); Distribution (mathematics); Boundary (topology)","score_opus":0.008056600018220856,"score_gpt":0.22871947753445204,"score_spread":0.22066287751623118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2968122134","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99908435,0.000116579526,0.00017558837,0.0000029683752,9.665288e-7,0.0000027043452,0.00013808718,0.0000058904693,0.00047278398],"genre_scores_gemma":[0.99929345,0.000041529613,0.00014887408,0.0000047903854,0.00000348914,0.000002342768,0.00029369068,0.0000021273206,0.00020973239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990153,0.000008198834,0.0000064888554,0.00003647266,0.000019794412,0.0000275465],"domain_scores_gemma":[0.9996636,0.000052812364,0.00010205384,0.000026091508,0.000060405826,0.00009512709],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013935927,0.00011220146,0.0001286721,0.0008826715,0.00021673822,0.0004508905,0.0001465591,0.00011339851,0.0011666851],"category_scores_gemma":[0.0002712146,0.000111729976,0.00009849985,0.0002611684,0.00018625044,0.00015569973,0.00031223008,0.00010678741,0.0002548618],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025102537,0.000050398347,0.7667263,0.000034739973,0.00009511425,0.00018093426,0.00039615564,0.00019997843,0.22444049,0.0001773511,0.00016258223,0.007284916],"study_design_scores_gemma":[0.0000045879233,0.000058370864,0.9923096,0.0000023838907,0.000010967717,0.0002050788,0.00010844898,0.00018643243,0.0066601858,0.000037200138,0.00041440633,0.0000024229978],"about_ca_topic_score_codex":0.00128707,"about_ca_topic_score_gemma":0.001400755,"teacher_disagreement_score":0.00128707,"about_ca_system_score_codex":0.00010648429,"about_ca_system_score_gemma":0.00005997857,"threshold_uncertainty_score":0.0039029121},"labels":[],"label_agreement":null},{"id":"W2968138885","doi":"10.3847/1538-4357/ab3126","title":"The Intrinsic Scatter of the Radial Acceleration Relation*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Spiral galaxy; Galaxy; Monte Carlo method; Galaxy rotation curve; Stellar mass; Scaling; Modified Newtonian dynamics","score_opus":0.006004724626990313,"score_gpt":0.19768496436968028,"score_spread":0.19168023974268997,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2968138885","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.46825376,0.00039082384,0.5228042,0.00039561806,0.00005468776,0.000060020895,0.0007222045,0.001181129,0.006137564],"genre_scores_gemma":[0.98236257,0.00007815988,0.01628511,0.000044326072,0.000022649541,0.000033744887,0.00032783754,0.000108005974,0.0007376418],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99802643,0.00086229795,0.00010531009,0.0005449462,0.0003148257,0.00014623898],"domain_scores_gemma":[0.99039865,0.004897501,0.0010257352,0.0026913055,0.00083285733,0.00015399011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004045504,0.00041103343,0.00053894665,0.00089754246,0.00040381995,0.001198959,0.0013247385,0.00049957173,0.0021445355],"category_scores_gemma":[0.01598179,0.0005276255,0.00071638124,0.0006023702,0.0008363107,0.001373174,0.00071457255,0.0007498383,0.0005751693],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011852114,0.00007686991,0.12880859,0.000054510954,0.0002462332,0.00015530948,0.00017442407,0.7962569,0.00489114,0.043423697,0.0010879331,0.02470585],"study_design_scores_gemma":[0.0000070413294,0.00002032981,0.012455223,0.000013831582,0.000018746032,0.000077986624,0.0000073911524,0.9745876,0.0019284416,0.01019821,0.0006619109,0.0000232129],"about_ca_topic_score_codex":0.0071568433,"about_ca_topic_score_gemma":0.005621385,"teacher_disagreement_score":0.0071568433,"about_ca_system_score_codex":0.0010812151,"about_ca_system_score_gemma":0.0006260453,"threshold_uncertainty_score":0.021394908},"labels":[],"label_agreement":null},{"id":"W2968337629","doi":"10.3847/1538-4357/abdcb7","title":"A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":237,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Kavli Foundation; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; Science and Engineering Research Board; National Science Foundation; Royal Society","keywords":"LIGO; Hubble's law; Galaxy; Neutron star; Sky; Cosmology; Dark energy; Binary number","score_opus":0.022221733639607198,"score_gpt":0.2868099657642753,"score_spread":0.2645882321246681,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2968337629","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98784465,0.00007531095,0.004977273,0.00021154659,0.00003180132,0.000018068009,0.002747769,0.00024059936,0.0038528456],"genre_scores_gemma":[0.99292046,0.000019889885,0.0026931143,0.000043082782,0.000024453431,0.000009961712,0.003044234,0.000039094433,0.0012056982],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992937,0.00017601434,0.000016178337,0.00017782167,0.00021197574,0.00012431463],"domain_scores_gemma":[0.99776614,0.00044521707,0.0005481462,0.0004700656,0.0003954529,0.0003749543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015976104,0.00028083308,0.00032841077,0.001315825,0.00028649767,0.0008526434,0.00034393175,0.00034015052,0.00095940864],"category_scores_gemma":[0.0043821265,0.00022693537,0.00029923295,0.00089571415,0.0002896288,0.00031590427,0.0011638524,0.0005337699,0.00047273882],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007712508,0.00012106506,0.93641824,0.000032332468,0.00024835585,0.00017929322,0.00038531734,0.0057547023,0.013543291,0.002958502,0.005345955,0.03424162],"study_design_scores_gemma":[0.000034796947,0.00010387766,0.97483873,0.00000858445,0.0000499293,0.000089624344,0.00006523003,0.016166907,0.004165603,0.0007166031,0.0037213096,0.00003883065],"about_ca_topic_score_codex":0.02156415,"about_ca_topic_score_gemma":0.0383728,"teacher_disagreement_score":0.02156415,"about_ca_system_score_codex":0.0008088582,"about_ca_system_score_gemma":0.00043447784,"threshold_uncertainty_score":0.042877257},"labels":[],"label_agreement":null},{"id":"W2969289116","doi":"10.3847/1538-4357/ab3d25","title":"Cloud Atlas: Variability in and out of the Water Band in the Planetary-mass HD 203030B Points to Cloud Sedimentation in Low-gravity L Dwarfs","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Western University","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration","keywords":"Brown dwarf; Physics; Astrophysics; Opacity; Amplitude; Astronomy; Planet","score_opus":0.0070856213623704065,"score_gpt":0.2197630334651155,"score_spread":0.2126774121027451,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969289116","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976185,0.00004083712,0.00015895122,0.00001805097,0.0000038646167,0.0000025804684,0.0013505385,0.0000515069,0.0007551227],"genre_scores_gemma":[0.9982285,0.000010977113,0.00020322338,0.000011306484,0.0000033675876,0.0000028905442,0.0014054686,0.0000074375944,0.00012684328],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999503,0.0000044413136,0.0000028729091,0.000013912826,0.000011338392,0.00001719398],"domain_scores_gemma":[0.9996768,0.000032235672,0.000103065264,0.00002382931,0.0000500948,0.00011397899],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014498108,0.00010692896,0.00013950458,0.0007916511,0.0002869824,0.00032527235,0.00016159957,0.00013596917,0.00092990935],"category_scores_gemma":[0.00031991862,0.000060897775,0.00013150093,0.00052163657,0.00013230779,0.00011578976,0.00019068131,0.00012482572,0.00034207586],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018548897,0.00003559544,0.9653063,0.000015968777,0.000025281446,0.00011563992,0.00017192906,0.0001888536,0.026766723,0.000090119145,0.0012101083,0.0058879983],"study_design_scores_gemma":[0.000001452168,0.0000066299926,0.9987834,9.874341e-7,0.0000029953337,0.00003645519,0.000023161527,0.00030396468,0.0006767063,0.000014518045,0.00014872149,9.550663e-7],"about_ca_topic_score_codex":0.017279776,"about_ca_topic_score_gemma":0.029679654,"teacher_disagreement_score":0.017279776,"about_ca_system_score_codex":0.0003847213,"about_ca_system_score_gemma":0.00016146942,"threshold_uncertainty_score":0.034358382},"labels":[],"label_agreement":null},{"id":"W2969316081","doi":"10.3847/1538-4357/ab3dae","title":"New Spatially Resolved Imaging of the SR 21 Transition Disk and Constraints on the Small-grain Disk Geometry","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Millimeter; Spectral energy distribution; Sublimation (psychology); Protoplanetary disk; RADIUS; Thin disk; Thick disk; Submillimeter Array","score_opus":0.007408087748569909,"score_gpt":0.2092163626015351,"score_spread":0.20180827485296518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969316081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938916,0.0003888879,0.0022180958,0.00005295999,0.000009077502,0.0000079777865,0.00026078188,0.00017718029,0.0029934326],"genre_scores_gemma":[0.9965928,0.0000540853,0.0026971514,0.000027996,0.00001230573,0.000005047762,0.00025746954,0.00001930307,0.00033376785],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99991786,0.0000058276223,0.0000040167797,0.000029884426,0.000019742456,0.000022588476],"domain_scores_gemma":[0.9995881,0.00007077655,0.00010796244,0.000078467085,0.00007346015,0.00008134563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019510256,0.00016383843,0.00021394508,0.0006996005,0.00020670018,0.00046137115,0.00038526027,0.00030574598,0.0019792223],"category_scores_gemma":[0.0003922227,0.00020044493,0.0002694663,0.00022052287,0.00020877697,0.00033246985,0.00041507513,0.00031156966,0.00041244156],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036198768,0.00006630526,0.041289553,0.00013440326,0.00007887601,0.0009130605,0.00021588018,0.0011783068,0.941637,0.0004908329,0.000562564,0.013071245],"study_design_scores_gemma":[0.00005234482,0.00031057632,0.898893,0.000042235817,0.00013003149,0.0039988854,0.0003388091,0.010766601,0.07698228,0.0006573089,0.0077836923,0.000044245116],"about_ca_topic_score_codex":0.0008850591,"about_ca_topic_score_gemma":0.0018300853,"teacher_disagreement_score":0.0019792223,"about_ca_system_score_codex":0.00024971014,"about_ca_system_score_gemma":0.000108064705,"threshold_uncertainty_score":0.006621182},"labels":[],"label_agreement":null},{"id":"W2969325082","doi":"10.3847/1538-4357/ab4f71","title":"Spallation-altered Accreted Compositions for X-Ray Bursts: Impact on Ignition Conditions and Burst Ashes","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"National Aeronautics and Space Administration; U.S. Department of Energy; National Nuclear Security Administration; National Science Foundation","keywords":"Spallation; Accretion (finance); Neutron star; Nucleosynthesis; Thermal; Atmosphere (unit); Nuclear reaction; Ignition system","score_opus":0.012114737687088189,"score_gpt":0.26826388633279236,"score_spread":0.25614914864570415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969325082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99403316,0.00013695432,0.003534004,0.00008370588,0.000011178286,0.000015098798,0.00032674812,0.000067995126,0.0017912022],"genre_scores_gemma":[0.9988607,0.0000668577,0.00045044266,0.000008109105,0.000003221487,0.000011207524,0.000119874916,0.000027875169,0.00045169276],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998841,0.000032923057,0.000008670699,0.000025763771,0.000020779822,0.000027685814],"domain_scores_gemma":[0.9992213,0.00031107324,0.00021260377,0.00006215089,0.000059737275,0.00013303148],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052158156,0.0006123331,0.00041420868,0.00047147446,0.0003296712,0.00095997966,0.000934284,0.00086013775,0.0029246914],"category_scores_gemma":[0.0017906366,0.0003979689,0.00070209143,0.00029414217,0.0005540638,0.0006168763,0.0006597998,0.0004581321,0.00029202862],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017568968,0.000064740096,0.019731907,0.000036689948,0.000041131258,0.00019328539,0.000029218516,0.9694462,0.007986245,0.0012437965,0.00009033679,0.000960757],"study_design_scores_gemma":[0.000030510766,0.00005400996,0.00790328,0.0000054745697,0.000018690778,0.000043382333,0.000025823523,0.9889904,0.0021729637,0.0006081611,0.00013541455,0.000011837537],"about_ca_topic_score_codex":0.0063057058,"about_ca_topic_score_gemma":0.0029463924,"teacher_disagreement_score":0.0063057058,"about_ca_system_score_codex":0.0009496106,"about_ca_system_score_gemma":0.0004003215,"threshold_uncertainty_score":0.012537956},"labels":[],"label_agreement":null},{"id":"W2969699193","doi":"10.3847/1538-4357/ab791d","title":"A Search for IceCube Events in the Direction of ANITA Neutrino Candidates","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Physics; Neutrino; Astrophysics; Flux (metallurgy); Solar neutrino problem; Astronomy; Neutrino detector; Solar neutrino; Neutrino oscillation; Particle physics","score_opus":0.016452427399301254,"score_gpt":0.2517908505624531,"score_spread":0.23533842316315184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969699193","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9834073,0.00031059093,0.0027640094,0.00015258377,0.000033767436,0.00004043661,0.003829037,0.00017042953,0.009291801],"genre_scores_gemma":[0.9826262,0.00023037569,0.0051720915,0.00007864645,0.00005618196,0.000055868546,0.010763729,0.00004633512,0.0009704425],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954444,0.00008193511,0.000018305642,0.00014891404,0.00012478215,0.0000816328],"domain_scores_gemma":[0.9982529,0.000628178,0.00058929727,0.0001763898,0.00016296814,0.00019023601],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00082567876,0.00041492263,0.00051859877,0.0014759923,0.0007146472,0.0013374501,0.00040104767,0.0005170193,0.002455434],"category_scores_gemma":[0.0013596935,0.00019223226,0.0005623874,0.0012828014,0.00032521563,0.00033501396,0.0009725022,0.000493469,0.0004703227],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0024348178,0.00024185357,0.87591076,0.00020279092,0.0005970904,0.0016101453,0.0007388372,0.005421429,0.069188714,0.0062046126,0.0054603345,0.031988505],"study_design_scores_gemma":[0.00016486549,0.00034084904,0.91143304,0.00007829367,0.00030028005,0.0014253972,0.00051545096,0.021884317,0.039333872,0.0026399505,0.021814309,0.00006944722],"about_ca_topic_score_codex":0.002427705,"about_ca_topic_score_gemma":0.004191596,"teacher_disagreement_score":0.002455434,"about_ca_system_score_codex":0.0005042989,"about_ca_system_score_gemma":0.00040932116,"threshold_uncertainty_score":0.008214295},"labels":[],"label_agreement":null},{"id":"W2969728939","doi":"10.3847/1538-4357/ab6d70","title":"Pressure Profiles and Mass Estimates Using High-resolution Sunyaev–Zel’dovich Effect Observations of Zwicky 3146 with MUSTANG-2","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Astronomical Observatory of Japan; Princeton University; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Science Foundation; Korea Astronomy and Space Science Institute; Office of Naval Research; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Virial theorem; Galaxy cluster; Intracluster medium; Sunyaev–Zel'dovich effect; Hydrostatic equilibrium; Planck; Cluster (spacecraft); Substructure; Galaxy; Astronomy","score_opus":0.012835944212891484,"score_gpt":0.2151154810343234,"score_spread":0.2022795368214319,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969728939","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989969,0.000035553294,0.00027738797,0.000012234262,9.732182e-7,0.0000040443083,0.00019111288,0.000011546451,0.0004702412],"genre_scores_gemma":[0.9992079,0.000013370028,0.00032872046,0.0000031882807,0.0000014698638,0.000003886561,0.00030905532,0.0000044463277,0.00012808554],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987113,0.000007926435,0.000007640347,0.00003762831,0.000044060598,0.00003154222],"domain_scores_gemma":[0.99974364,0.000032417753,0.000110511646,0.00003332594,0.00002947656,0.000050667528],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020776401,0.0002159692,0.00020592962,0.0012742486,0.00036582167,0.00041170127,0.00037697426,0.00019144446,0.00077282975],"category_scores_gemma":[0.0004892682,0.00019497109,0.00018467307,0.00066052994,0.00026982263,0.00023097027,0.0008579011,0.00017829273,0.00020064761],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019232336,0.000020143796,0.948862,0.000016387225,0.000060728424,0.00019311254,0.00033588495,0.0013786287,0.042657536,0.00026934626,0.00023790137,0.0057760957],"study_design_scores_gemma":[0.0000049218247,0.0000071083373,0.996801,0.000001920944,0.0000072085945,0.000024181962,0.000033395267,0.0009906726,0.0018476826,0.000028833829,0.00024937125,0.0000036849196],"about_ca_topic_score_codex":0.016221749,"about_ca_topic_score_gemma":0.031292826,"teacher_disagreement_score":0.016221749,"about_ca_system_score_codex":0.0007049553,"about_ca_system_score_gemma":0.00013658979,"threshold_uncertainty_score":0.032254696},"labels":[],"label_agreement":null},{"id":"W2969759531","doi":"10.3847/1538-4357/ab7afb","title":"ANTARES and IceCube Combined Search for Neutrino Point-like and Extended Sources in the Southern Sky","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Villum Fonden; Institut Universitaire de France; Japan Society for the Promotion of Science; Institut National de Physique Nucléaire et de Physique des Particules; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; Bundesministerium für Bildung und Forschung; Natural Sciences and Engineering Research Council of Canada; Knut och Alice Wallenbergs Stiftelse; College of Engineering, Michigan State University; Marsden Fund; Helmholtz Alliance for Astroparticle Physics; Conseil Régional d'Alsace; Istituto Nazionale di Fisica Nucleare; Junta de Andalucía; Chiba University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Vetenskapsrådet; Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii; Centre National de la Recherche Scientifique; Conseil Régional, Île-de-France; Fonds Wetenschappelijk Onderzoek; Danmarks Grundforskningsfond; Polarforskningssekretariatet; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; National Science Foundation; Belgian Federal Science Policy Office; Fonds De La Recherche Scientifique - FNRS; Marquette University; Ministerio de Ciencia, Innovación y Universidades; Western Canada Research Grid; National Research Foundation; Conseil Régional Provence-Alpes-Côte d'Azur; Office of Polar Programs; Michigan State University; University of Oxford; Compute Canada; Labex UnivEarthS; U.S. Department of Energy; University of Wisconsin-Madison; European Commission; Deutsches Elektronen-Synchrotron; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Generalitat Valenciana; National Research Foundation of Korea","keywords":"Sky; Neutrino; Cosmic ray; COSMIC cancer database; Supernova; Neutrino astronomy; Flux (metallurgy)","score_opus":0.013406739520298363,"score_gpt":0.23028923395726683,"score_spread":0.21688249443696847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2969759531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9476202,0.00082067144,0.0075675617,0.00018472479,0.000035255915,0.0001605177,0.022008907,0.0007266313,0.020875655],"genre_scores_gemma":[0.87929463,0.00050203135,0.046241134,0.000090412286,0.00008533865,0.0001989648,0.068767056,0.00017346026,0.004647007],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993956,0.00014442648,0.00001772199,0.00014817313,0.000219943,0.00007405552],"domain_scores_gemma":[0.9992694,0.00014948739,0.00015813306,0.000119742836,0.00019182556,0.00011147548],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011986301,0.00048275746,0.0006666213,0.0027970804,0.000328268,0.0009041697,0.00043128338,0.0002693484,0.002288769],"category_scores_gemma":[0.0006483464,0.0002931869,0.0006763148,0.0023165662,0.00017472266,0.00034478793,0.0010732915,0.00021409708,0.0007746716],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.008911077,0.00045762502,0.6637607,0.00036443875,0.0019322791,0.0012492416,0.00043677088,0.03809598,0.124720864,0.0037528845,0.020773659,0.1355444],"study_design_scores_gemma":[0.00046244124,0.00068075146,0.891498,0.00008483399,0.00051028124,0.0009951625,0.00036872757,0.03327794,0.031573024,0.0017742551,0.038704574,0.000069984344],"about_ca_topic_score_codex":0.00860178,"about_ca_topic_score_gemma":0.024524564,"teacher_disagreement_score":0.00860178,"about_ca_system_score_codex":0.0003541003,"about_ca_system_score_gemma":0.0006242129,"threshold_uncertainty_score":0.017103434},"labels":[],"label_agreement":null},{"id":"W2970053044","doi":"10.3847/1538-4357/ab564b","title":"A Search for MeV to TeV Neutrinos from Fast Radio Bursts with IceCube","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Neutrino; Flux (metallurgy); Range (aeronautics); Neutrino detector; Neutrino astronomy","score_opus":0.014646028499435028,"score_gpt":0.2322595846058801,"score_spread":0.21761355610644506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2970053044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96361524,0.0008059867,0.0047808336,0.00048012892,0.00008178375,0.00009598857,0.0070626675,0.00032077217,0.022756608],"genre_scores_gemma":[0.9762708,0.00038824975,0.009474652,0.000291158,0.00014172423,0.000110480876,0.011424247,0.00009521568,0.0018034372],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999308,0.0001466347,0.000027644806,0.00019226814,0.00018120633,0.0001443031],"domain_scores_gemma":[0.9975189,0.0009114182,0.0006422258,0.00031325268,0.00029000547,0.00032418605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014141976,0.00054468605,0.0006221789,0.002013175,0.000791699,0.0016561846,0.0005290991,0.00061146996,0.0025121374],"category_scores_gemma":[0.0017940712,0.00033005455,0.000497952,0.0021668463,0.00039414142,0.00045543615,0.0012054851,0.00045173737,0.0004619303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0036785165,0.00044671964,0.8493116,0.00020091422,0.00077032944,0.0016058728,0.00069653656,0.0095397765,0.049963504,0.007136559,0.013652521,0.062997185],"study_design_scores_gemma":[0.0003069897,0.0006208129,0.8866987,0.00014541473,0.00032472695,0.0016754708,0.00078274123,0.026981058,0.030248763,0.0031942038,0.048927337,0.000093650546],"about_ca_topic_score_codex":0.005018592,"about_ca_topic_score_gemma":0.0070014717,"teacher_disagreement_score":0.005018592,"about_ca_system_score_codex":0.0008419164,"about_ca_system_score_gemma":0.00083180045,"threshold_uncertainty_score":0.009978771},"labels":[],"label_agreement":null},{"id":"W2970854026","doi":"10.3847/1538-4357/ab3e76","title":"KFPA Examinations of Young STellar Object Natal Environments (KEYSTONE): Hierarchical Ammonia Structures in Galactic Giant Molecular Clouds","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; University of Alberta; University of Victoria","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Virial theorem; Molecular cloud; Virial mass; Mean kinetic temperature; Young stellar object; Star formation; Galaxy; Kinetic energy; Green Bank Telescope; Velocity dispersion; Protein filament; Milky Way; Stars; Chemistry","score_opus":0.005239095914555284,"score_gpt":0.22062496512289492,"score_spread":0.21538586920833963,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2970854026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99910104,0.000026101632,0.00004410891,0.000006283856,3.9305047e-7,0.0000021641952,0.00023316528,0.000002540971,0.0005843256],"genre_scores_gemma":[0.9990054,0.00002955953,0.00016422659,0.000010333286,0.0000015097348,0.0000040400873,0.0005369949,0.0000021391236,0.00024585056],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986935,0.000016491587,0.000009206637,0.000032678734,0.000029702387,0.00004255259],"domain_scores_gemma":[0.99949837,0.00006426713,0.00015892713,0.000052195017,0.000105650935,0.00012058044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023313407,0.00012071224,0.000106543506,0.0011439404,0.00047394418,0.00036766243,0.00016080674,0.00012412565,0.00082220533],"category_scores_gemma":[0.0005204116,0.00007269631,0.00014443135,0.0005411372,0.00023958358,0.00029570158,0.0006939751,0.0000894768,0.00016762974],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000028099399,0.0000044717867,0.9930489,0.0000042359593,0.0000123514965,0.000069045294,0.00023460436,0.000076446726,0.0048669716,0.00004200504,0.000057311947,0.0015554271],"study_design_scores_gemma":[3.7426582e-7,0.000005090187,0.99921286,0.0000010912775,0.0000022341942,0.000037610494,0.00014172492,0.00005124939,0.0003975712,0.000011413842,0.00013793408,7.987345e-7],"about_ca_topic_score_codex":0.01923999,"about_ca_topic_score_gemma":0.04917376,"teacher_disagreement_score":0.01923999,"about_ca_system_score_codex":0.00043322597,"about_ca_system_score_gemma":0.000214472,"threshold_uncertainty_score":0.03825599},"labels":[],"label_agreement":null},{"id":"W2970858640","doi":"10.3847/1538-4357/ab6d67","title":"Search for PeV Gamma-Ray Emission from the Southern Hemisphere with 5 Yr of Data from the IceCube Observatory","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Cosmic ray; Air shower; Observatory; Galactic plane; Southern Hemisphere; Neutrino; Flux (metallurgy); Muon","score_opus":0.04391613580762971,"score_gpt":0.2535743848456383,"score_spread":0.20965824903800862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2970858640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99285114,0.0003117378,0.002429447,0.000045433146,0.0000034357377,0.000019292795,0.0021819633,0.00009906293,0.0020584548],"genre_scores_gemma":[0.98682797,0.00013164124,0.004277268,0.000041984957,0.000010714514,0.000024156976,0.0081448555,0.000038542483,0.00050295633],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962854,0.000120501754,0.00002119577,0.000087646746,0.000076489145,0.00006559826],"domain_scores_gemma":[0.99917656,0.00025709093,0.00026282875,0.0000876209,0.00010735742,0.0001085321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009878931,0.0004181951,0.0004568162,0.0011707308,0.0004177839,0.000750141,0.0003994476,0.0003465951,0.0014188982],"category_scores_gemma":[0.0011782,0.0002781707,0.00049431383,0.00075202016,0.00015318536,0.00033271083,0.00043550474,0.00023659985,0.00024759828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005630895,0.00006268333,0.95955235,0.000057335026,0.00037929782,0.00027070407,0.00011780787,0.004960753,0.019679856,0.00019203886,0.0006704321,0.013493671],"study_design_scores_gemma":[0.000039668445,0.00014425658,0.9769338,0.000027191743,0.000086809516,0.00030824993,0.00009182642,0.011717922,0.0068883086,0.00015669108,0.0035918446,0.000013514489],"about_ca_topic_score_codex":0.0069801537,"about_ca_topic_score_gemma":0.014846942,"teacher_disagreement_score":0.0069801537,"about_ca_system_score_codex":0.0005007161,"about_ca_system_score_gemma":0.0002841742,"threshold_uncertainty_score":0.013879061},"labels":[],"label_agreement":null},{"id":"W2971380221","doi":"10.3847/1538-4357/ab3231","title":"Erratum: “Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015–2017 LIGO Data” (2019, ApJ, 879, 10)","year":2019,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Physics; Astrophysics; LIGO; Amplitude; Glitch; Vela; Table (database); Astronomy; Gravitational wave; Detector; Computer science; Optics","score_opus":0.0466732771727982,"score_gpt":0.3702462695738758,"score_spread":0.3235729924010776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2971380221","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00170526,0.0019524909,0.0018170741,0.046618473,0.87509096,0.000048853744,0.03885667,0.0022283639,0.031681813],"genre_scores_gemma":[0.027047507,0.0076616188,0.011126967,0.06251475,0.09767528,0.00026433603,0.11936444,0.008373239,0.6659718],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9972639,0.00020855328,0.0006308391,0.00033206065,0.0013787705,0.0001858704],"domain_scores_gemma":[0.98738503,0.002135826,0.001298474,0.0009953952,0.00749809,0.00068714604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020873353,0.0016330199,0.0010247539,0.0066151614,0.003971491,0.00455289,0.0013157869,0.0022228758,0.07970021],"category_scores_gemma":[0.029700754,0.0007392076,0.00089077617,0.005834587,0.0015781929,0.0030436171,0.002819128,0.004843874,0.09187745],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000021091333,0.0000048337347,0.00020136808,0.000042633423,0.0000039792853,0.00005307971,0.000028372966,0.00001836896,0.00003980821,0.0005139129,0.99496776,0.004104831],"study_design_scores_gemma":[0.000018974477,0.000017284534,0.0024106405,0.00025326002,0.000020118097,0.00018040412,0.00014468837,0.00008517512,0.00027055098,0.0009836318,0.99558264,0.000032566757],"about_ca_topic_score_codex":0.035373945,"about_ca_topic_score_gemma":0.039839953,"teacher_disagreement_score":0.07970021,"about_ca_system_score_codex":0.0037348205,"about_ca_system_score_gemma":0.0054642474,"threshold_uncertainty_score":0.26662374},"labels":[],"label_agreement":null},{"id":"W2971437851","doi":"10.3847/1538-4357/ab425c","title":"A Rapidly Declining Transient Discovered with the Subaru/Hyper Suprime-Cam","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Russian Science Foundation; Russian Foundation for Basic Research; Ministry of Education, Culture, Sports, Science and Technology; Toyota Foundation","keywords":"Supergiant; Brightness; Red supergiant; Apparent magnitude; Transient (computer programming); Stars; Circumstellar envelope; Supernova; Stellar evolution","score_opus":0.00862288121925396,"score_gpt":0.2436461735615856,"score_spread":0.23502329234233166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2971437851","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965836,0.000052239473,0.0008782358,0.00002269336,0.000005698256,0.000019750754,0.00042054532,0.00010341739,0.0019138627],"genre_scores_gemma":[0.99548316,0.000022318653,0.0031323934,0.00003674288,0.000014200784,0.000016947395,0.00092716725,0.000026602333,0.00034038824],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998547,0.00001422709,0.0000070501915,0.00004085222,0.000037997856,0.00004512735],"domain_scores_gemma":[0.99939406,0.00005705235,0.00014314592,0.00012392808,0.00007598747,0.00020579346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042103973,0.00021975423,0.00029799796,0.0009665374,0.0004803826,0.00046085712,0.0003829114,0.00026502353,0.00086890283],"category_scores_gemma":[0.0003228413,0.0002072976,0.00030646301,0.0005976793,0.00019765053,0.00021738104,0.00065744994,0.00029471848,0.0002644357],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010607268,0.00029842334,0.7473599,0.000070357215,0.00019418895,0.0016076446,0.0005846697,0.0016612167,0.20680396,0.0004996854,0.0018433258,0.03801585],"study_design_scores_gemma":[0.000017795852,0.00023855886,0.98903733,0.000005989447,0.00003558955,0.0004509007,0.000105173676,0.0024832708,0.0060481927,0.00006153916,0.00150411,0.00001162271],"about_ca_topic_score_codex":0.0023001595,"about_ca_topic_score_gemma":0.005588761,"teacher_disagreement_score":0.0023001595,"about_ca_system_score_codex":0.0002763117,"about_ca_system_score_gemma":0.0002242352,"threshold_uncertainty_score":0.004573524},"labels":[],"label_agreement":null},{"id":"W2971721367","doi":"10.3847/1538-4357/ab418b","title":"Compact Star-forming Galaxies as Old Starbursts Becoming Quiescent","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"University of Toronto; National Research Foundation; Danmarks Grundforskningsfond; Villum Fonden","keywords":"Physics; Astrophysics; Galaxy; Star (game theory); Astronomy; Star formation; Luminous infrared galaxy","score_opus":0.009679967340725546,"score_gpt":0.22894533665775477,"score_spread":0.21926536931702922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2971721367","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989266,0.00031156387,0.00008259038,0.000025076639,0.0000027463784,0.0000024126425,0.00007410913,0.000009595936,0.0005652849],"genre_scores_gemma":[0.99966145,0.000077079465,0.000031122316,0.0000072586827,0.0000051099273,8.7887923e-7,0.000059176815,0.000001104643,0.00015680648],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987257,0.000019218558,0.000011001685,0.000035301782,0.000017110482,0.000044758013],"domain_scores_gemma":[0.9977449,0.0004025646,0.00088405696,0.00012614744,0.00015044447,0.0006918453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032162783,0.00013978782,0.00020362354,0.0012633499,0.00025579197,0.0011568498,0.00023496887,0.00032375703,0.0020870962],"category_scores_gemma":[0.0017612986,0.00011366386,0.00014237048,0.00070249167,0.0005858227,0.00070812873,0.000400799,0.00028002536,0.00026406406],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001809755,0.000044531942,0.98471296,0.000018454342,0.000021753156,0.00032130527,0.0010868352,0.00015988709,0.005641514,0.0005297274,0.00014246417,0.0071395244],"study_design_scores_gemma":[0.000003266848,0.000040596664,0.99857664,0.0000041185212,0.000007781962,0.00037467424,0.00024184329,0.00014964811,0.00015286112,0.0001762677,0.00027049746,0.0000017838206],"about_ca_topic_score_codex":0.0023520645,"about_ca_topic_score_gemma":0.0018876861,"teacher_disagreement_score":0.0023520645,"about_ca_system_score_codex":0.0002158749,"about_ca_system_score_gemma":0.000106930485,"threshold_uncertainty_score":0.0069820285},"labels":[],"label_agreement":null},{"id":"W2971932552","doi":"10.3847/1538-4357/ab4266","title":"No Sign of G2's Encounter Affecting Sgr A*'s X-Ray Flaring Rate from Chandra Observations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; McGill University Health Centre","funders":"Fonds de recherche du Québec – Nature et technologies; McGill Space Institute; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; McGill University; Canadian Institute for Advanced Research","keywords":"Physics; Astrophysics; Sign (mathematics); Astronomy; X-ray; Nuclear physics","score_opus":0.014702792160666745,"score_gpt":0.22004956261299102,"score_spread":0.20534677045232427,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2971932552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968951,0.000040559193,0.00044302232,0.000048580834,0.000007664403,0.000008558002,0.0011180878,0.00011309784,0.0013254678],"genre_scores_gemma":[0.997678,0.000010438472,0.000251818,0.00002212397,0.0000056348076,0.0000032832609,0.0018749449,0.000022333754,0.00013149017],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99941134,0.000091162714,0.00003591233,0.00021488174,0.00012502758,0.00012179216],"domain_scores_gemma":[0.9982059,0.00046928154,0.00039738667,0.00033617936,0.00019901658,0.0003922187],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007923012,0.00036345632,0.00030775453,0.000657632,0.00043757795,0.001422445,0.00048086958,0.0005609745,0.0019119622],"category_scores_gemma":[0.00311218,0.00015606149,0.0006772565,0.0005880783,0.00040518117,0.00057561893,0.0006368825,0.0004953527,0.00047332278],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049411034,0.00008419958,0.9763208,0.000063732106,0.00026871345,0.00041167595,0.00017839456,0.007922438,0.0077025155,0.00042329106,0.0015118471,0.0046181567],"study_design_scores_gemma":[0.00001919301,0.00012886112,0.9777796,0.000012851583,0.00007356703,0.0003494174,0.00028579685,0.017513184,0.002352997,0.00021896929,0.0012432648,0.000022304832],"about_ca_topic_score_codex":0.011076391,"about_ca_topic_score_gemma":0.0112931365,"teacher_disagreement_score":0.011076391,"about_ca_system_score_codex":0.00041989938,"about_ca_system_score_gemma":0.00035753206,"threshold_uncertainty_score":0.022023857},"labels":[],"label_agreement":null},{"id":"W2972009598","doi":"10.3847/1538-4357/ab3e3a","title":"A Simplified, Lossless Reanalysis of PAPER-64","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":139,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Advanced Research","funders":"","keywords":"Reionization; Spectral density; Estimator; Redshift; Physics; Astrophysics; Sidereal time; Algorithm; Computer science; Galaxy; Mathematics; Statistics","score_opus":0.006228033206179582,"score_gpt":0.21438711840439592,"score_spread":0.20815908519821633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972009598","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.62962717,0.0011154511,0.21713462,0.0014058294,0.001178113,0.00017443467,0.050632868,0.024464497,0.07426699],"genre_scores_gemma":[0.84095275,0.0005989576,0.093733445,0.0004236562,0.0002776691,0.00013903972,0.033335496,0.0054837177,0.025055373],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993895,0.00004917157,0.000031315976,0.00014941185,0.0003092194,0.00007128594],"domain_scores_gemma":[0.9988789,0.00014174079,0.00017312917,0.0004248695,0.00034574242,0.000035613877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007836531,0.0008362532,0.00048791946,0.0033779973,0.00045006172,0.0025661965,0.0012741964,0.00057106663,0.008228654],"category_scores_gemma":[0.0030387898,0.00062953983,0.0010425528,0.0034866785,0.00030870514,0.00181614,0.00095800427,0.0009335543,0.0041447375],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008752614,0.00027841944,0.20518982,0.00051820127,0.0012207462,0.0017593085,0.0014646663,0.14933263,0.13243587,0.031301644,0.054124966,0.42149845],"study_design_scores_gemma":[0.000119351855,0.00014736371,0.47692353,0.00010107953,0.0003393832,0.00076741975,0.0004926594,0.27025437,0.04497094,0.022685055,0.18289068,0.00030825028],"about_ca_topic_score_codex":0.009971588,"about_ca_topic_score_gemma":0.008841549,"teacher_disagreement_score":0.009971588,"about_ca_system_score_codex":0.0008482986,"about_ca_system_score_gemma":0.0006586686,"threshold_uncertainty_score":0.02752763},"labels":[],"label_agreement":null},{"id":"W2972096190","doi":"10.3847/1538-4357/ab418f","title":"A New Technique for Finding Galaxies Leaking Lyman-continuum Radiation: [S ii]-deficiency","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":75,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Astronomy","score_opus":0.00816255123487005,"score_gpt":0.2268977077409379,"score_spread":0.21873515650606784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972096190","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8628883,0.0013510461,0.1250555,0.0005107906,0.00008382195,0.0005186308,0.0015684027,0.0024932802,0.005530342],"genre_scores_gemma":[0.80205554,0.0006770454,0.19239011,0.0002675584,0.000091190734,0.0003631479,0.0010861505,0.00007261594,0.0029966848],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99972695,0.000050453942,0.000017673845,0.00009445168,0.000068865884,0.00004164136],"domain_scores_gemma":[0.99905235,0.00028567895,0.00022476145,0.0001719602,0.000099504905,0.00016581503],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005286711,0.00037208517,0.00033730347,0.002807442,0.0004432719,0.0004236723,0.000591372,0.00056218053,0.0025649164],"category_scores_gemma":[0.0005963376,0.00022908454,0.00036648175,0.0009043343,0.00052520627,0.00066752115,0.00087253214,0.0005359159,0.00055696175],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067956914,0.00032784187,0.21302553,0.00032484726,0.0001732001,0.0007240337,0.0008834379,0.0003588115,0.66358846,0.0010177253,0.001325401,0.1175712],"study_design_scores_gemma":[0.0002385759,0.0031714644,0.72899634,0.000045324017,0.00031215226,0.011547235,0.0009285279,0.007156738,0.23053874,0.0017645377,0.01515494,0.0001453305],"about_ca_topic_score_codex":0.001181022,"about_ca_topic_score_gemma":0.0024768123,"teacher_disagreement_score":0.002807442,"about_ca_system_score_codex":0.00014292898,"about_ca_system_score_gemma":0.00024520297,"threshold_uncertainty_score":0.008580446},"labels":[],"label_agreement":null},{"id":"W2972139276","doi":"10.3847/1538-4357/ab3424","title":"Evidence for the Cross-correlation between Cosmic Microwave Background Polarization Lensing from Polarbear and Cosmic Shear from Subaru Hyper Suprime-Cam","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; National Central University; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; National Energy Research Scientific Computing Center; Agence Nationale de la Recherche; Space Telescope Science Institute; Eötvös Loránd Tudományegyetem; Academia Sinica; Labex UnivEarthS; Japan Science and Technology Agency; Smithsonian Institution; U.S. Department of Energy; European Commission; Johns Hopkins University; Princeton University; Queen's University Belfast; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Durham University; National Science Foundation","keywords":"Cosmic microwave background; Amplitude; COSMIC cancer database; Galaxy; Observational cosmology; Polarization (electrochemistry); Cosmology; Cosmic background radiation; Weak gravitational lensing","score_opus":0.027723118809857228,"score_gpt":0.28626095102024024,"score_spread":0.258537832210383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972139276","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99630105,0.00017921397,0.0010303427,0.00006784825,0.000012698088,0.0000030095923,0.0005577712,0.000037235506,0.0018107522],"genre_scores_gemma":[0.99833834,0.000058809168,0.00049749686,0.000022174174,0.000026077354,0.0000033856704,0.00094542664,0.000015060725,0.0000933079],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99933136,0.00017695964,0.000030484653,0.00019966705,0.00018071181,0.000080824175],"domain_scores_gemma":[0.9952461,0.0014232948,0.0015914249,0.0007419802,0.00056895893,0.00042808012],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012077919,0.0005551488,0.00024585726,0.0014774983,0.00030608664,0.0007470994,0.00031288507,0.00030737303,0.0013547926],"category_scores_gemma":[0.0037845368,0.00029566578,0.00030170512,0.0014959031,0.0004690069,0.00027800075,0.00091099687,0.0004030099,0.00035036844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018990786,0.000019667745,0.98250717,0.000019112216,0.00020830004,0.00015675776,0.00012369978,0.0003772199,0.010456569,0.00038371293,0.00035556755,0.005202282],"study_design_scores_gemma":[0.00000294487,0.000018719777,0.9978728,0.0000028176141,0.000029657358,0.000074039206,0.000023819655,0.00056069857,0.0010761599,0.00010329888,0.00022956335,0.0000053867884],"about_ca_topic_score_codex":0.0036611403,"about_ca_topic_score_gemma":0.006286848,"teacher_disagreement_score":0.0036611403,"about_ca_system_score_codex":0.00020251371,"about_ca_system_score_gemma":0.00017661846,"threshold_uncertainty_score":0.0072796345},"labels":[],"label_agreement":null},{"id":"W2972254451","doi":"10.3847/1538-4357/ab3124","title":"Polycyclic Aromatic Hydrocarbons with Armchair Edges: Potential Emitters in Class B Sources","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Spectral line; Class (philosophy); Aromaticity; Molecule; Quantum mechanics","score_opus":0.004998459364665108,"score_gpt":0.19950369784528663,"score_spread":0.1945052384806215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972254451","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9912777,0.00047928214,0.006423846,0.000034061974,0.0000034359634,0.000013441645,0.000118016564,0.000044513232,0.0016056567],"genre_scores_gemma":[0.9967879,0.0002018885,0.0024739092,0.000019525714,0.0000043497434,0.000006717183,0.00018733561,0.0000125607385,0.00030568824],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999926,0.0000121898165,0.0000031746583,0.000021559388,0.000019843943,0.000017262122],"domain_scores_gemma":[0.9996934,0.00011923856,0.00007723483,0.000023344182,0.000037893267,0.000048963975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002867425,0.00033259825,0.00020824038,0.0007125166,0.0003203572,0.00049532816,0.00028585023,0.00041180587,0.0011993891],"category_scores_gemma":[0.00060041476,0.00016247237,0.00033864853,0.0005562092,0.00018800364,0.00055817765,0.00040818998,0.000313042,0.00016471562],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008110626,0.00030452287,0.6443963,0.00042602728,0.0004110453,0.0011471193,0.00033781753,0.0861004,0.19013515,0.015471881,0.00072944176,0.05972927],"study_design_scores_gemma":[0.00013109484,0.00070318766,0.45691827,0.00013013036,0.00043811614,0.0011737898,0.00093713886,0.40862018,0.10178354,0.020049006,0.008968546,0.00014715723],"about_ca_topic_score_codex":0.001491841,"about_ca_topic_score_gemma":0.0020193262,"teacher_disagreement_score":0.001491841,"about_ca_system_score_codex":0.00021402177,"about_ca_system_score_gemma":0.0001809606,"threshold_uncertainty_score":0.0040123463},"labels":[],"label_agreement":null},{"id":"W2972335439","doi":"10.3847/1538-4357/ab7921","title":"Intermediate-mass Black Holes’ Effects on Compact Object Binaries","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Supermassive black hole; Merge (version control); Star cluster; Galactic Center; Population; Black hole (networking); Binary number","score_opus":0.01423521448541279,"score_gpt":0.2361058982553954,"score_spread":0.22187068376998262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972335439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99655366,0.00011505175,0.0007366206,0.000062155144,0.000012059856,0.0000060105763,0.000054649136,0.000031459127,0.002428268],"genre_scores_gemma":[0.9996489,0.0000240214,0.00009464249,0.000011750842,0.000003068444,0.0000015822374,0.000020848887,0.000008942682,0.00018612012],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999001,0.000029351424,0.000004308609,0.000014707398,0.000016420561,0.000035077268],"domain_scores_gemma":[0.9993326,0.00026287956,0.00010916935,0.000058033944,0.00004889904,0.00018845887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041716185,0.00039246265,0.0005923717,0.00040486688,0.00084046763,0.001033689,0.00056424295,0.00050075527,0.0035522357],"category_scores_gemma":[0.0016655744,0.00021094721,0.0004700327,0.0002540033,0.0009680986,0.0010364694,0.0011764051,0.00050284644,0.00027422293],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011323013,0.00055206905,0.09998636,0.00016606814,0.00029313902,0.0013554598,0.0004583634,0.83830994,0.025612416,0.021949844,0.001107355,0.009076729],"study_design_scores_gemma":[0.00019692665,0.00033709974,0.045592025,0.000025322428,0.00008663305,0.00016668075,0.0002720863,0.93955404,0.006069983,0.006775431,0.00087767513,0.000046143527],"about_ca_topic_score_codex":0.0065411422,"about_ca_topic_score_gemma":0.0034908724,"teacher_disagreement_score":0.0065411422,"about_ca_system_score_codex":0.0007917228,"about_ca_system_score_gemma":0.0003375336,"threshold_uncertainty_score":0.013006091},"labels":[],"label_agreement":null},{"id":"W2972355550","doi":"10.3847/1538-4357/ab8945","title":"Discovery and Rapid Follow-up Observations of the Unusual Type II SN 2018ivc in NGC 1068","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Israel Science Foundation; National Natural Science Foundation of China; National Aeronautics and Space Administration","keywords":"Supernova; Ejecta; Light curve; Pair-instability supernova; Spectral line; Hubble space telescope; Spitzer Space Telescope","score_opus":0.025329557985600715,"score_gpt":0.2294647872298014,"score_spread":0.2041352292442007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972355550","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997724,0.0001226854,0.00027224078,0.000034802983,0.000010986999,0.000012257269,0.00049853063,0.000037767506,0.0012867898],"genre_scores_gemma":[0.9978259,0.000045391433,0.0006271893,0.000023093116,0.000014161683,0.0000088214265,0.001038013,0.0000066686507,0.00041074754],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987185,0.000007201925,0.000008040966,0.0000340671,0.000047178823,0.00003168681],"domain_scores_gemma":[0.9995666,0.000032326872,0.00012997648,0.00005026931,0.00010146181,0.00011942099],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019740587,0.00020062849,0.00023145613,0.0010643014,0.0004942083,0.00038156044,0.0003248472,0.00031959853,0.00074127875],"category_scores_gemma":[0.0004966564,0.00014443687,0.00014767898,0.00040981802,0.0001815427,0.00016622063,0.0005208106,0.00041014512,0.00030705112],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025656592,0.000119486525,0.9059741,0.00003228511,0.000049910344,0.0036720736,0.0002718859,0.00017512018,0.06647341,0.00015981578,0.001078427,0.021737024],"study_design_scores_gemma":[0.0000066688076,0.00012733773,0.9918759,0.000009331018,0.000014727738,0.0025195698,0.000095547075,0.0003185322,0.002271171,0.000054092787,0.002700441,0.00000669798],"about_ca_topic_score_codex":0.004514149,"about_ca_topic_score_gemma":0.0094018495,"teacher_disagreement_score":0.004514149,"about_ca_system_score_codex":0.0003793634,"about_ca_system_score_gemma":0.0001124772,"threshold_uncertainty_score":0.008975744},"labels":[],"label_agreement":null},{"id":"W2972364776","doi":"10.3847/1538-4357/ab441f","title":"Weighing the Darkness: Astrometric Mass Measurement of Hidden Stellar Companions Using Gaia","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Seventh Framework Programme; University of Crete; Danmarks Grundforskningsfond; FP7 Research Potential of Convergence Regions; National Research Foundation; European Commission","keywords":"Physics; Astrometry; White dwarf; Astronomy; Astrophysics; Brown dwarf; Neutron star; Orbit (dynamics); Binary number; Stars; Orbital period; Binary star; Measure (data warehouse)","score_opus":0.026508444959533015,"score_gpt":0.23513903761677804,"score_spread":0.20863059265724504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972364776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897189,0.00018195556,0.006862987,0.000050386916,0.000019813033,0.000014201876,0.00052743603,0.00029199652,0.002332336],"genre_scores_gemma":[0.9940222,0.0000254011,0.005512862,0.000020297965,0.000005152211,0.000004034417,0.00024844377,0.000016415768,0.00014530096],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998056,0.00003756328,0.000008869158,0.000078802004,0.000037664508,0.000031489388],"domain_scores_gemma":[0.9989502,0.00013105304,0.00036868968,0.00026780213,0.00015630148,0.00012593456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004891134,0.00026817917,0.00022375745,0.0013835733,0.00033887022,0.0006783647,0.00037499378,0.0002654109,0.00054494257],"category_scores_gemma":[0.002107375,0.00016260176,0.00020432952,0.0006770148,0.00031214172,0.0006755547,0.0008981541,0.0002803283,0.00030147855],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044129963,0.00005602341,0.9121937,0.00005160981,0.00018328702,0.00012089627,0.00039711606,0.0074739186,0.042536464,0.0016980298,0.00090509874,0.03394256],"study_design_scores_gemma":[0.000019139794,0.00017217241,0.9050123,0.000034182023,0.00009601408,0.00034838094,0.0002782404,0.06422955,0.024234856,0.0019188756,0.0036129265,0.000043404616],"about_ca_topic_score_codex":0.0025864635,"about_ca_topic_score_gemma":0.0053958646,"teacher_disagreement_score":0.0025864635,"about_ca_system_score_codex":0.00040565516,"about_ca_system_score_gemma":0.00017498544,"threshold_uncertainty_score":0.0051428676},"labels":[],"label_agreement":null},{"id":"W2972575927","doi":"10.3847/1538-4357/ab43c8","title":"An ALMA Study of the FU Ori–type Object V900 Mon: Implications for the Progenitor","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Astronomical Observatory of Japan; European Commission; National Institutes of Natural Sciences; Russian Foundation for Basic Research; European Space Agency; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Astrophysics; Physics; Outflow; Stars; Astronomy; Young stellar object; Emission spectrum; Accretion (finance); Star formation; Protostar; Spectral line","score_opus":0.016687497333793447,"score_gpt":0.28509836392029886,"score_spread":0.2684108665865054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2972575927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979603,0.00017611105,0.00024325281,0.0000264362,0.0000035128896,0.0000036275615,0.00010856759,0.00001364891,0.0014644227],"genre_scores_gemma":[0.9992343,0.000041579737,0.00030045124,0.000016696298,0.000010904026,0.0000018283608,0.00017994706,0.0000033988395,0.0002108442],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999325,0.000004983709,0.0000030610477,0.000022818705,0.000015748354,0.000020833333],"domain_scores_gemma":[0.999795,0.000021134563,0.000069095964,0.000022685193,0.000025165575,0.00006685179],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017582702,0.00017543348,0.0002413529,0.0006303173,0.0005326218,0.00065612013,0.0003453724,0.00032870207,0.0007871088],"category_scores_gemma":[0.00027481496,0.00013887098,0.00017871261,0.0005164787,0.00024252495,0.0003834537,0.00035280958,0.00022012857,0.00022280667],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042497934,0.00017580658,0.7889885,0.00006511125,0.00007105274,0.0025086734,0.0006294999,0.00074877794,0.18632162,0.0008332003,0.00043292856,0.0187999],"study_design_scores_gemma":[0.0000062233594,0.00010106487,0.9924575,0.0000075388516,0.00001950894,0.0007353228,0.0002178457,0.0016421142,0.0025958652,0.00013824341,0.0020714584,0.0000072490957],"about_ca_topic_score_codex":0.005187557,"about_ca_topic_score_gemma":0.0072053047,"teacher_disagreement_score":0.005187557,"about_ca_system_score_codex":0.0006762326,"about_ca_system_score_gemma":0.00012218367,"threshold_uncertainty_score":0.010314763},"labels":[],"label_agreement":null},{"id":"W2973088614","doi":"10.3847/1538-4357/ab2fce","title":"A Recipe for Finding Stellar Radii, Temperatures, Surface Gravities, Metallicities, and Masses Using Spectral Lines","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Recipe; Effective temperature; Surface gravity; Astrophysics; RADIUS; Parallax; Angular diameter; Luminosity; Photosphere; Stars; Interferometry; Stellar classification; Astronomy; Spectral line; Galaxy","score_opus":0.020223321022030782,"score_gpt":0.24888726136284514,"score_spread":0.22866394034081436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2973088614","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.006158901,0.0001347637,0.95579296,0.00012288221,0.0001336344,0.00047091843,0.0027351128,0.031558968,0.0028918262],"genre_scores_gemma":[0.015800245,0.00007245198,0.974725,0.000065091,0.000024518265,0.00043751783,0.0014848094,0.0047219982,0.0026684063],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99893683,0.00017178134,0.00012372923,0.00023084776,0.0004881576,0.000048750207],"domain_scores_gemma":[0.99614656,0.0010660039,0.00037405555,0.0008346436,0.0014306753,0.0001480842],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002133038,0.001701951,0.0011509,0.0039001524,0.0011111965,0.0014448913,0.0020269675,0.00076938386,0.031246968],"category_scores_gemma":[0.015620329,0.0020591954,0.0014166259,0.0012865014,0.00063589995,0.0015985059,0.0013333877,0.0017164749,0.023227263],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003779767,0.00027701273,0.0210256,0.0017602696,0.000503666,0.00084229687,0.0007554067,0.024828266,0.15176879,0.032241683,0.1067392,0.6588798],"study_design_scores_gemma":[0.00024350846,0.00031173055,0.03388252,0.00021122798,0.00019890186,0.0017275292,0.0003088239,0.32368913,0.20925067,0.05661649,0.37278163,0.00077779574],"about_ca_topic_score_codex":0.0024252026,"about_ca_topic_score_gemma":0.0036602516,"teacher_disagreement_score":0.031246968,"about_ca_system_score_codex":0.0006438887,"about_ca_system_score_gemma":0.00097138266,"threshold_uncertainty_score":0.10453147},"labels":[],"label_agreement":null},{"id":"W2974309548","doi":"10.3847/1538-4357/ab45e9","title":"The ALMA Survey of 70 μm Dark High-mass Clumps in Early Stages (ASHES). I. Pilot Survey: Clump Fragmentation","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":190,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"IBM (Canada)","funders":"","keywords":"Physics; Astrophysics; Fragmentation (computing); High mass; Mass distribution; Star formation; Stars","score_opus":0.016641589235781847,"score_gpt":0.2541505028679489,"score_spread":0.23750891363216703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2974309548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99859756,0.00009704459,0.0001761672,0.000020089812,0.0000026169125,0.000021667542,0.0005744276,0.000024565352,0.0004858993],"genre_scores_gemma":[0.9966774,0.0000715409,0.0009932214,0.000037186568,0.000017235849,0.00002568178,0.001613348,0.000010094702,0.00055439485],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975556,0.000032619784,0.00001304996,0.00004650057,0.0000628158,0.00008952882],"domain_scores_gemma":[0.9984768,0.00011609758,0.00035740013,0.00016304603,0.00024471837,0.00064186234],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057523535,0.00023400683,0.0002881385,0.0017707743,0.000470725,0.00046863375,0.0005488552,0.00026786717,0.00088718423],"category_scores_gemma":[0.0007352936,0.00018380035,0.00027184238,0.00060565735,0.00018613753,0.00032230682,0.00089355797,0.0002565117,0.0003407115],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026303242,0.0001027885,0.9738153,0.000027177499,0.00003648009,0.0003354906,0.00034468024,0.000121931036,0.012135547,0.000111981906,0.0010074744,0.011697958],"study_design_scores_gemma":[0.000017156122,0.00007827311,0.99748224,0.0000047019926,0.0000082802235,0.00012134615,0.00012022628,0.00031012253,0.0007104494,0.000022974555,0.0011204649,0.0000037950356],"about_ca_topic_score_codex":0.0071720555,"about_ca_topic_score_gemma":0.017144684,"teacher_disagreement_score":0.0071720555,"about_ca_system_score_codex":0.0003783083,"about_ca_system_score_gemma":0.00023833141,"threshold_uncertainty_score":0.01426059},"labels":[],"label_agreement":null},{"id":"W2974454386","doi":"10.3847/1538-4357/ab43cb","title":"Radiative Association of Atomic and Ionic Carbon","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Fullerene Chemistry and Applications","field":"Chemistry","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Gauss Centre for Supercomputing; Queen's University; Office of Science; Queen's University Belfast; National Energy Research Scientific Computing Center; Institute for Theoretical Atomic, Molecular and Optical Physics, Harvard University; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Radiative transfer; Ionic bonding; Potential energy; Dipole; Carbon fibers; Atom (system on chip); Coupling (piping)","score_opus":0.0036494183939708488,"score_gpt":0.20085797192879967,"score_spread":0.19720855353482883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2974454386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97711164,0.00025248496,0.012536719,0.00007450377,0.00003794148,0.00003927623,0.00014610658,0.00008065941,0.009720721],"genre_scores_gemma":[0.99798137,0.00005649563,0.00065502716,0.000016659944,0.0000040377436,0.000009312544,0.00009076251,0.000019896564,0.0011665162],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99937326,0.00008775263,0.00002404624,0.0001223141,0.0001864644,0.00020614272],"domain_scores_gemma":[0.9984282,0.00082052517,0.00022591885,0.00016655907,0.00023812318,0.00012068728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012558487,0.0005894458,0.00058277394,0.00080689054,0.0010823172,0.000786225,0.0011738228,0.0006368455,0.0059946673],"category_scores_gemma":[0.0027471492,0.0003121307,0.0006296458,0.0007017456,0.0007409923,0.0010230596,0.0010044436,0.0006190868,0.0003354264],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009571692,0.00039941462,0.04378114,0.0006057681,0.00035392185,0.0012766053,0.00086258916,0.7224745,0.09221436,0.11799137,0.001010975,0.018072233],"study_design_scores_gemma":[0.00012330794,0.00036125755,0.01166211,0.000034124343,0.00011684954,0.0005463726,0.0002887936,0.86174583,0.11253261,0.010292473,0.0021785798,0.0001176165],"about_ca_topic_score_codex":0.0047710543,"about_ca_topic_score_gemma":0.0037653707,"teacher_disagreement_score":0.0059946673,"about_ca_system_score_codex":0.0013741879,"about_ca_system_score_gemma":0.0010760834,"threshold_uncertainty_score":0.020054221},"labels":[],"label_agreement":null},{"id":"W2974467107","doi":"10.3847/1538-4357/ab4657","title":"CLOVER: Convnet Line-fitting Of Velocities in Emission-line Regions","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Alberta; University of Victoria","funders":"","keywords":"Line (geometry); Pixel; Noise (video); Physics; Artificial intelligence; Spectral line; Emission spectrum; Algorithm; Pattern recognition (psychology); Computer science; Astrophysics; Mathematics; Geometry; Image (mathematics); Astronomy","score_opus":0.01167419980379153,"score_gpt":0.26229857441059007,"score_spread":0.25062437460679854,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2974467107","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22195299,0.0022591937,0.5222357,0.0011572737,0.0010340693,0.00050930434,0.017097827,0.21825981,0.01549387],"genre_scores_gemma":[0.54193336,0.0005140454,0.37247488,0.0020848725,0.00018240638,0.00056723884,0.057334654,0.0055711716,0.019337412],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99970406,0.00002018636,0.000011421598,0.00015595366,0.000052043462,0.000056196353],"domain_scores_gemma":[0.9996263,0.00008626919,0.000045725992,0.000090522015,0.00011427667,0.000036834208],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005038175,0.0034239097,0.0008030694,0.000978805,0.00056396954,0.0011059385,0.0036563464,0.0017215336,0.007540276],"category_scores_gemma":[0.0016339794,0.0009841176,0.0010870093,0.0008866109,0.0005244978,0.0017512977,0.00094553205,0.0017592425,0.0039408617],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091061555,0.0005741614,0.006720086,0.00036510456,0.00038469702,0.00035130332,0.00012405784,0.50144994,0.019446906,0.0034859492,0.1547514,0.31143573],"study_design_scores_gemma":[0.000029650935,0.000031337346,0.00034502443,0.000010020039,0.000010162508,0.00003039055,0.000015806683,0.99105376,0.0049198084,0.0010801532,0.0024602315,0.000013696305],"about_ca_topic_score_codex":0.043466054,"about_ca_topic_score_gemma":0.063093714,"teacher_disagreement_score":0.043466054,"about_ca_system_score_codex":0.00185487,"about_ca_system_score_gemma":0.0013851408,"threshold_uncertainty_score":0.08642614},"labels":[],"label_agreement":null},{"id":"W2975040766","doi":"10.3847/1538-4357/ab3c2d","title":"Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during Their First and Second Observing Runs","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Institut des Origines de Lyon; Ministero dello Sviluppo Economico; Ministry of Education, India; National Research Foundation of Korea; Engineering and Physical Sciences Research Council; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; European Commission; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Science and Engineering Research Board; National Science Foundation; Royal Society","keywords":"LIGO; Binary black hole; Eccentricity (behavior); Binary number; Eccentric; Waveform; Orbital eccentricity","score_opus":0.007843075844124851,"score_gpt":0.26242143605400853,"score_spread":0.25457836020988367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2975040766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990533,0.0000349535,0.0003539015,0.0000147146175,0.000001371219,0.000009666541,0.00020929241,0.000030880878,0.00029193226],"genre_scores_gemma":[0.9982071,0.000012349171,0.0009315965,0.000009181046,0.000004205799,0.000009136884,0.0006713651,0.000009568672,0.00014549305],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993437,0.00012258164,0.000028435907,0.00019307615,0.00015628703,0.00015581289],"domain_scores_gemma":[0.99756855,0.0006717411,0.00070801127,0.00026732156,0.00017326899,0.00061109755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012576986,0.00037714807,0.0005288684,0.0025680817,0.0004403917,0.00078774925,0.0005354188,0.0005256279,0.0006693431],"category_scores_gemma":[0.0025300088,0.00027680476,0.0003664381,0.001153887,0.00033789745,0.0004672893,0.0013253783,0.0003917896,0.00016535373],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046109542,0.000104226805,0.97246855,0.000021362417,0.00012862193,0.00017040288,0.00028642386,0.0016467643,0.015611852,0.00018934331,0.00017642174,0.008734926],"study_design_scores_gemma":[0.000023121618,0.00016439984,0.99309385,0.0000044303542,0.00003320653,0.00012470258,0.00008820165,0.0037811156,0.002220282,0.000052047464,0.0004025149,0.000012239812],"about_ca_topic_score_codex":0.004698551,"about_ca_topic_score_gemma":0.010969412,"teacher_disagreement_score":0.004698551,"about_ca_system_score_codex":0.0005066738,"about_ca_system_score_gemma":0.00032635673,"threshold_uncertainty_score":0.009342372},"labels":[],"label_agreement":null},{"id":"W2975061125","doi":"10.3847/1538-4357/ab3d3c","title":"The Implications of Local Fluctuations in the Galactic Midplane for Dynamical Analysis in the Gaia Era","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Milky Way; Orbit (dynamics); Galactic Center; Systematic error; Galactic plane; Variation (astronomy); Disc","score_opus":0.008564782221783704,"score_gpt":0.24914076965462903,"score_spread":0.24057598743284533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2975061125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98834527,0.0007420149,0.004060987,0.0009904724,0.000053504562,0.0000068993754,0.00056230836,0.000120447505,0.0051182257],"genre_scores_gemma":[0.99832445,0.00009840096,0.00089098676,0.000041412648,0.000025729765,0.000003811942,0.0002055681,0.000051552197,0.00035811545],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99960047,0.00011842403,0.00003076178,0.00012664193,0.00006523682,0.000058589885],"domain_scores_gemma":[0.9979108,0.0009049271,0.00035364175,0.00036559466,0.00027778596,0.00018718427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013907241,0.00017390194,0.00027681745,0.0010084251,0.0004995091,0.0018372944,0.0005864914,0.00025203242,0.0016664523],"category_scores_gemma":[0.009274162,0.00013895376,0.00041367678,0.0009817773,0.0006463705,0.00089546293,0.00096262567,0.00048906397,0.00032343867],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036919644,0.00003987205,0.8733994,0.00010117819,0.0003478291,0.00060417305,0.0013366971,0.031172557,0.007698447,0.028285064,0.002321495,0.054324143],"study_design_scores_gemma":[0.000010610797,0.000040154908,0.9376737,0.000036008874,0.00006168338,0.00014561595,0.00045801135,0.04869715,0.0017929791,0.0062665027,0.0047909264,0.000026648971],"about_ca_topic_score_codex":0.014240854,"about_ca_topic_score_gemma":0.010090339,"teacher_disagreement_score":0.014240854,"about_ca_system_score_codex":0.0012248415,"about_ca_system_score_gemma":0.00034815987,"threshold_uncertainty_score":0.028315961},"labels":[],"label_agreement":null},{"id":"W2975282412","doi":"10.3847/1538-4357/ab4b48","title":"Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Istituto Nazionale di Fisica Nucleare; Leverhulme Trust; Scottish Funding Council; Russian Science Foundation; Ministry of Education, India; National Research Foundation of Korea; Engineering and Physical Sciences Research Council; Hungarian Scientific Research Fund; Generalitat Valenciana; Council of Scientific and Industrial Research, India; Centre National de la Recherche Scientifique; Industry Canada; Kavli Foundation; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; Science and Engineering Research Board; National Science Foundation; Royal Society","keywords":"LIGO; Physics; Gravitational wave; Neutron star; Gamma-ray burst; Astrophysics; Fermi Gamma-ray Space Telescope; Redshift; Astronomy; Binary number; Gravitational-wave astronomy; Galaxy","score_opus":0.011974816426275335,"score_gpt":0.28358769855297933,"score_spread":0.271612882126704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2975282412","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99827874,0.000051696006,0.0007776003,0.000017971319,0.0000023593211,0.0000065626073,0.0004404513,0.000050607858,0.0003740625],"genre_scores_gemma":[0.9977266,0.000025069123,0.0005976903,0.000008389388,0.0000038973635,0.0000072234543,0.0014448555,0.000010181574,0.00017606089],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995931,0.000089041394,0.000017758044,0.00011186616,0.00010929887,0.000079035395],"domain_scores_gemma":[0.99888307,0.00024501578,0.00044510848,0.00016280715,0.00009311527,0.00017086272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008992699,0.0005069473,0.0004008139,0.0010708194,0.0002608173,0.00078437856,0.0003963947,0.00038480732,0.0006879131],"category_scores_gemma":[0.001642524,0.00023982882,0.00072451227,0.0005265132,0.00025421093,0.0003721501,0.00082662574,0.00027896825,0.00020201558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052183995,0.00007254284,0.9640908,0.000036040965,0.0004189778,0.00014903503,0.00012720925,0.010866286,0.01720377,0.00047351784,0.00026191009,0.0057781013],"study_design_scores_gemma":[0.000029881885,0.0002562172,0.9652857,0.000011153815,0.0001124277,0.00018253396,0.000079748505,0.0261433,0.006699908,0.00024430658,0.0009291298,0.000025713525],"about_ca_topic_score_codex":0.004981303,"about_ca_topic_score_gemma":0.01083132,"teacher_disagreement_score":0.004981303,"about_ca_system_score_codex":0.0006439513,"about_ca_system_score_gemma":0.0004052814,"threshold_uncertainty_score":0.009904623},"labels":[],"label_agreement":null},{"id":"W2975825974","doi":"10.3847/1538-4357/ab3c1a","title":"The Analogous Structure of Accretion Flows in Supermassive and Stellar Mass Black Holes: New Insights from Faded Changing-look Quasars","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Quasar; Supermassive black hole; Active galactic nucleus; Accretion (finance); Intermediate-mass black hole; Black hole (networking); Binary black hole; Binary number","score_opus":0.0075670526814912015,"score_gpt":0.2072610945940207,"score_spread":0.19969404191252949,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2975825974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989697,0.00010815701,0.00036465345,0.000020151148,0.0000022830293,0.0000028772663,0.00007805324,0.0000143307925,0.00043982395],"genre_scores_gemma":[0.9995511,0.000039534945,0.00024427247,0.000011859658,0.0000063032917,0.0000014488628,0.000076222175,0.000004013473,0.00006519727],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999399,0.0000069330645,0.0000034383827,0.000018946652,0.000009108145,0.000021629752],"domain_scores_gemma":[0.9994228,0.00013318894,0.00022267373,0.000056964935,0.00005292078,0.0001115181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021058509,0.00015113153,0.00025012283,0.0015596264,0.00022286725,0.0007221351,0.0002771412,0.00019865452,0.0008825824],"category_scores_gemma":[0.0007138481,0.00017603504,0.00021218842,0.0005260645,0.0005885067,0.00052113907,0.0005728801,0.00044160197,0.00008716505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031482778,0.00015373506,0.87693745,0.00006952438,0.00009727883,0.0009624418,0.0015726527,0.0011840517,0.104398146,0.0020043538,0.0002237233,0.012081779],"study_design_scores_gemma":[0.000003257608,0.00002015448,0.9971187,0.0000044281333,0.000006909984,0.00013842035,0.00021288583,0.0010631753,0.00081004767,0.0004562504,0.00015992703,0.00000597376],"about_ca_topic_score_codex":0.0017557908,"about_ca_topic_score_gemma":0.0017733881,"teacher_disagreement_score":0.0017557908,"about_ca_system_score_codex":0.00024103529,"about_ca_system_score_gemma":0.00008487317,"threshold_uncertainty_score":0.0034911036},"labels":[],"label_agreement":null},{"id":"W2975911227","doi":"10.3847/1538-4357/ab9633","title":"Quenching as a Contest between Galaxy Halos and Their Central Black Holes","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Simon Fraser University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Halo; Astronomy; Peculiar galaxy; Galaxy formation and evolution; Stellar mass; Star formation; Disc","score_opus":0.011872617092017985,"score_gpt":0.20955568471612737,"score_spread":0.1976830676241094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2975911227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9609186,0.0004440433,0.011525491,0.0011920524,0.000020620697,0.000014844274,0.00004214991,0.00018516394,0.025656965],"genre_scores_gemma":[0.9991517,0.000021759517,0.00028740033,0.0000270292,0.000010504067,0.0000019308304,0.000007641129,0.000008811895,0.00048318738],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99968493,0.000089559384,0.000010522551,0.00006072943,0.00006640348,0.00008796999],"domain_scores_gemma":[0.99741095,0.0007290184,0.000650507,0.00037386804,0.00020303196,0.0006325944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011836963,0.00014843018,0.0002949065,0.00045244006,0.0008254762,0.001964799,0.00061807304,0.00052706804,0.0051250076],"category_scores_gemma":[0.00454995,0.00017729016,0.00030674276,0.00026304112,0.004207559,0.0019279858,0.0019127075,0.00074311625,0.00019399477],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023534821,0.000038792572,0.032457788,0.0000441866,0.000025290688,0.0002281419,0.0018427517,0.011274898,0.0059039267,0.93264157,0.000938455,0.0143688815],"study_design_scores_gemma":[0.00007844102,0.00013890307,0.06569678,0.000030077734,0.000025261965,0.00022032647,0.00075664616,0.044483524,0.0016212944,0.8814259,0.005480026,0.000042804804],"about_ca_topic_score_codex":0.0030136527,"about_ca_topic_score_gemma":0.0012959971,"teacher_disagreement_score":0.0051250076,"about_ca_system_score_codex":0.0011774667,"about_ca_system_score_gemma":0.0003313576,"threshold_uncertainty_score":0.017144859},"labels":[],"label_agreement":null},{"id":"W2976009229","doi":"10.3847/1538-4357/ab5e8a","title":"Mitigating Internal Instrument Coupling for 21 cm Cosmology. II. A Method Demonstration with the Hydrogen Epoch of Reionization Array","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"FP7 International Cooperation; Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; National Research Foundation; Canadian Institute for Advanced Research; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"HERA; Physics; Reionization; Spectral density; Cosmology; Systematics; Astrophysics; Coupling (piping); Computer science; Particle physics; Telecommunications; Engineering; Galaxy","score_opus":0.015300357554940818,"score_gpt":0.24319867984776983,"score_spread":0.227898322292829,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2976009229","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2897452,0.00048577823,0.7032683,0.0010539846,0.000110794295,0.000096774755,0.00038601368,0.0016612386,0.0031919274],"genre_scores_gemma":[0.677418,0.00016789437,0.31977862,0.00020803032,0.00005709448,0.00011013187,0.0002972156,0.0003368237,0.0016261487],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99866354,0.0007432978,0.000037812377,0.00016356795,0.0003182544,0.000073557225],"domain_scores_gemma":[0.99346304,0.0021186075,0.0011681548,0.00258241,0.00052399514,0.0001437756],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0050074467,0.00062414154,0.00027060322,0.00040649693,0.0004213411,0.00070894277,0.00075365877,0.00043195215,0.0009031589],"category_scores_gemma":[0.0085540265,0.00032442718,0.0006256632,0.0004933101,0.0003900223,0.0007480736,0.0011927714,0.0008368954,0.00030976],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007897269,0.00030327233,0.26833472,0.00028347786,0.00083294144,0.00051262375,0.00091528974,0.11675528,0.13150264,0.05063168,0.004378446,0.42475986],"study_design_scores_gemma":[0.00014348711,0.0007849525,0.18902113,0.00010489355,0.00025520913,0.00078773126,0.00036632363,0.6360279,0.10407025,0.039524134,0.028686691,0.00022736228],"about_ca_topic_score_codex":0.002251104,"about_ca_topic_score_gemma":0.0050988602,"teacher_disagreement_score":0.0050074467,"about_ca_system_score_codex":0.0005257447,"about_ca_system_score_gemma":0.0008236102,"threshold_uncertainty_score":0.026482224},"labels":[],"label_agreement":null},{"id":"W2976448072","doi":"10.3847/1538-4357/ab4794","title":"Dwarf Galaxy Discoveries from the KMTNet Supernova Program. II. The NGC 3585 Group and Its Dynamical State*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Dwarf galaxy; Dwarf spheroidal galaxy; Interacting galaxy; Irregular galaxy; Galaxy; Galaxy group; Gravitational microlensing; Local Group; Lenticular galaxy","score_opus":0.005510677697749775,"score_gpt":0.2068237412016112,"score_spread":0.20131306350386144,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2976448072","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990194,0.00010591023,0.00013447953,0.0000086831515,0.0000023352786,0.000003110655,0.00023993832,0.000008069648,0.0004780621],"genre_scores_gemma":[0.9991898,0.000024906545,0.0001513894,0.0000044422463,0.0000024266521,0.0000012390663,0.0005084895,0.000001138585,0.000116292445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998474,0.000014369096,0.000012473781,0.00004582727,0.00004423651,0.000035590318],"domain_scores_gemma":[0.9997056,0.000020985563,0.000118893455,0.000027779939,0.00003407752,0.000092624345],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028147292,0.000141924,0.0001083341,0.0012541154,0.0002488704,0.000367575,0.00014705071,0.00007629081,0.00048439455],"category_scores_gemma":[0.00029978662,0.00005378688,0.00015544161,0.0005059328,0.00020217436,0.00016473744,0.00039555217,0.000097601136,0.000085547756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006996452,0.000010730737,0.9887115,0.000009339934,0.000021520142,0.0001437587,0.00010508549,0.00008869126,0.0052155186,0.00017656657,0.0001172642,0.005329955],"study_design_scores_gemma":[0.0000014948675,0.00002708202,0.99785966,0.000002723469,0.00001388109,0.00020878934,0.00006857435,0.00024447154,0.00083158404,0.00005089646,0.00068909914,0.0000018383906],"about_ca_topic_score_codex":0.004657095,"about_ca_topic_score_gemma":0.009008374,"teacher_disagreement_score":0.004657095,"about_ca_system_score_codex":0.00029963546,"about_ca_system_score_gemma":0.00014081728,"threshold_uncertainty_score":0.009259939},"labels":[],"label_agreement":null},{"id":"W2976493770","doi":"10.3847/1538-4357/ab75e2","title":"The Green Bank North Celestial Cap Pulsar Survey. V. Pulsar Census and Survey Sensitivity","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Pulsar; Sky; Population; Sensitivity (control systems); Millisecond pulsar; Flux (metallurgy); Pulse (music); Dispersion (optics)","score_opus":0.028736062294196143,"score_gpt":0.29732394314408184,"score_spread":0.2685878808498857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2976493770","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7172616,0.0030888363,0.0030675037,0.001136251,0.00015814546,0.00037887917,0.23345797,0.0009215249,0.040529277],"genre_scores_gemma":[0.82487965,0.0014482285,0.006263299,0.0010263466,0.00016851854,0.00043647902,0.15507966,0.00030496845,0.010392835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982534,0.0003853297,0.00010166439,0.00031729354,0.0006881735,0.00025419312],"domain_scores_gemma":[0.99221414,0.0013389589,0.001416788,0.0011986912,0.0029586956,0.00087278115],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026834654,0.00027621633,0.0004564725,0.0047609056,0.0006993532,0.0011291251,0.0005828117,0.00030454504,0.0046727033],"category_scores_gemma":[0.0072420277,0.00031864262,0.00019147329,0.0070890975,0.0003365823,0.00043302117,0.0010718242,0.00032279265,0.002431964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012016581,0.000025224323,0.9328015,0.000072352166,0.000049829647,0.00008149799,0.00019819493,0.0009881192,0.00067946344,0.00029187108,0.035877675,0.02881422],"study_design_scores_gemma":[0.000007724701,0.000007345334,0.99003285,0.00002144668,0.000005831288,0.000038893995,0.000055979217,0.0006757326,0.00013364822,0.000049283233,0.008965396,0.0000059406316],"about_ca_topic_score_codex":0.36126524,"about_ca_topic_score_gemma":0.43703282,"teacher_disagreement_score":0.36126524,"about_ca_system_score_codex":0.002080239,"about_ca_system_score_gemma":0.0016805216,"threshold_uncertainty_score":0.7183249},"labels":[],"label_agreement":null},{"id":"W2976514883","doi":"10.3847/0004-637x/827/1/2","title":"CONSTRAINTS ON THE DISTANCE MODULI, HELIUM AND METAL ABUNDANCES, AND AGES OF GLOBULAR CLUSTERS FROM THEIR RR LYRAE AND NON-VARIABLE HORIZONTAL-BRANCH STARS. I. M3, M15, AND M92","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"RR Lyrae variable; Globular cluster; Physics; Astrophysics; Horizontal branch; Metallicity; Stars; Instability strip; Variable star; Absolute magnitude; Luminosity; Population; Astronomy; Cepheid variable; Galaxy","score_opus":0.006787568017605358,"score_gpt":0.19325037678410217,"score_spread":0.18646280876649682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2976514883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99894947,0.00005151707,0.00024446743,0.000009998217,7.3197754e-7,0.0000015391438,0.00018392422,0.000007933211,0.0005505178],"genre_scores_gemma":[0.99922204,0.000015217558,0.0003091446,0.0000048899296,0.0000012319623,0.0000023806306,0.00037240968,0.000004971522,0.00006770635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999887,0.000017001146,0.000012282542,0.000038802387,0.000016537362,0.000028333418],"domain_scores_gemma":[0.99914896,0.00026395608,0.00020942188,0.000114015435,0.00009492048,0.00016871453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050415716,0.0004867142,0.00021903924,0.0006798248,0.00039901733,0.000555615,0.00039556384,0.000395473,0.0011206185],"category_scores_gemma":[0.0012125763,0.00021064049,0.0004674047,0.0005118613,0.0002563672,0.00036808453,0.00059609493,0.00021286096,0.0005268722],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034979818,0.0000203871,0.9753592,0.00002080493,0.00004568583,0.00007156692,0.00027183295,0.0035457013,0.013197407,0.0008497867,0.0002453657,0.006022501],"study_design_scores_gemma":[0.0000224472,0.00007205938,0.9876215,0.000012341634,0.000025477791,0.00007801083,0.00017078339,0.008475744,0.002188428,0.00062796095,0.00069721264,0.000007998821],"about_ca_topic_score_codex":0.0046955566,"about_ca_topic_score_gemma":0.0068747997,"teacher_disagreement_score":0.0046955566,"about_ca_system_score_codex":0.0005079826,"about_ca_system_score_gemma":0.00019729165,"threshold_uncertainty_score":0.009336472},"labels":[],"label_agreement":null},{"id":"W2976777994","doi":"10.3847/1538-4357/ab3c62","title":"T CrB: Radio Observations during the 2016–2017 “Super-active” State","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Aeronautics and Space Administration","keywords":"Bremsstrahlung; Ionization; Photoionization; Photosphere; Accretion (finance); Spectral energy distribution; Binary number; Emission spectrum; Binary system; Spectral line","score_opus":0.015815652676039575,"score_gpt":0.22521124716720406,"score_spread":0.2093955944911645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2976777994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948874,0.00007030554,0.00020015544,0.000073755145,0.000035643552,0.000017729313,0.0011334502,0.000042513784,0.003538939],"genre_scores_gemma":[0.995906,0.000042160376,0.0002837499,0.000040684135,0.0000501136,0.000013892891,0.0026189985,0.00001566498,0.0010287273],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977976,0.000015435859,0.000011480135,0.000042984648,0.00008118567,0.00006924122],"domain_scores_gemma":[0.9993812,0.000034715606,0.00013879173,0.000062300714,0.00016091588,0.00022202685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043741986,0.00016724752,0.00023556306,0.00078379834,0.0005919853,0.0005055204,0.0002822603,0.00037458577,0.0014538994],"category_scores_gemma":[0.00061476306,0.00010088221,0.00018456498,0.00048377202,0.00030340697,0.0002476136,0.0006915349,0.000510517,0.00070853677],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022867224,0.0005270525,0.76850027,0.00014351204,0.00015496468,0.0022181096,0.0020376192,0.00071202224,0.18095356,0.0007681187,0.006648636,0.03504932],"study_design_scores_gemma":[0.000015847836,0.00012686366,0.9936206,0.000008673088,0.000013041545,0.00020736217,0.00022123367,0.00029485856,0.0018296664,0.00003949907,0.0036154934,0.000006765193],"about_ca_topic_score_codex":0.012729243,"about_ca_topic_score_gemma":0.030055441,"teacher_disagreement_score":0.012729243,"about_ca_system_score_codex":0.00045646905,"about_ca_system_score_gemma":0.00040744976,"threshold_uncertainty_score":0.025310338},"labels":[],"label_agreement":null},{"id":"W2976920865","doi":"10.3847/1538-4357/ab48fc","title":"A Reanalysis of the Fundamental Parameters and Age of TRAPPIST-1*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Effective temperature; Astrophysics; Surface gravity; Spectral energy distribution; Stellar classification; Metallicity; Near-infrared spectroscopy; RADIUS; Brown dwarf; Stars; Optics","score_opus":0.009400290200457134,"score_gpt":0.20970474473935707,"score_spread":0.20030445453889995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2976920865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906668,0.00013500615,0.0014260084,0.00007005283,0.000015054053,0.000007896697,0.0052436213,0.00020376031,0.002231832],"genre_scores_gemma":[0.98775834,0.000099557736,0.0017542377,0.000027881835,0.000012257185,0.000008975454,0.008841508,0.00005322253,0.0014439464],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999567,0.0000012043467,0.0000012798849,0.000018718982,0.000012894934,0.000009137531],"domain_scores_gemma":[0.99972993,0.000017120754,0.000059445087,0.00003425211,0.00012588305,0.000033303055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014152654,0.00023740612,0.00013879049,0.0009307314,0.00032173606,0.00040824895,0.00029320395,0.0001642166,0.0013430018],"category_scores_gemma":[0.00039010783,0.000112728885,0.00021836904,0.00091988407,0.00010425766,0.00030860628,0.00025793829,0.0003346054,0.00049311284],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023970641,0.000052733703,0.8252178,0.00013109647,0.00016317058,0.0005136667,0.0005690058,0.011061879,0.03276389,0.00057241425,0.0073695173,0.12134505],"study_design_scores_gemma":[0.000008670989,0.000034569133,0.9735571,0.000013469575,0.000052497973,0.00025840825,0.00013962193,0.010385707,0.0025381339,0.00015048977,0.012849102,0.0000121249595],"about_ca_topic_score_codex":0.020923542,"about_ca_topic_score_gemma":0.03137649,"teacher_disagreement_score":0.020923542,"about_ca_system_score_codex":0.00063806877,"about_ca_system_score_gemma":0.0003534037,"threshold_uncertainty_score":0.041603506},"labels":[],"label_agreement":null},{"id":"W2977008301","doi":"10.3847/1538-4357/ab4269","title":"Constraints on the Galactic Inner Halo Assembly History from the Age Gradient of Blue Horizontal-branch Stars","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Milky Way; Halo; Physics; Astrophysics; Galactic halo; Metallicity; Astronomy; Galaxy; Galaxy formation and evolution; Population; Stars","score_opus":0.01353935319286558,"score_gpt":0.2050538669316843,"score_spread":0.1915145137388187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2977008301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990171,0.0001108366,0.0003040132,0.0000063244306,7.1737156e-7,8.0476843e-7,0.00019519887,0.00000975382,0.00035521464],"genre_scores_gemma":[0.99929774,0.000046317236,0.00016550781,0.0000033537058,0.0000018508845,7.335257e-7,0.00040948146,0.000004079745,0.000070824586],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985504,0.000025161902,0.000011746306,0.000040217692,0.00003481172,0.000032897464],"domain_scores_gemma":[0.99878246,0.0002568528,0.0003718724,0.00016868416,0.000204582,0.00021564521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004323058,0.00015845223,0.0001828599,0.001567947,0.00020554946,0.0007689338,0.00020827474,0.00017618014,0.0010650753],"category_scores_gemma":[0.001612447,0.00012646384,0.00024720884,0.00063354854,0.0002160827,0.00029793687,0.0005002836,0.00013437247,0.00036985116],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000067994246,0.000005251465,0.9864231,0.000008765118,0.000035932455,0.00002821385,0.000059298338,0.00048313636,0.008170542,0.00009497506,0.000046586876,0.004576205],"study_design_scores_gemma":[0.0000011095166,0.000011135666,0.9978527,0.0000031929785,0.0000102506165,0.00003084518,0.00003856427,0.0010492698,0.0007612496,0.000050437313,0.00018949335,0.0000017912351],"about_ca_topic_score_codex":0.00396903,"about_ca_topic_score_gemma":0.005930774,"teacher_disagreement_score":0.00396903,"about_ca_system_score_codex":0.00020070387,"about_ca_system_score_gemma":0.00012784169,"threshold_uncertainty_score":0.007891893},"labels":[],"label_agreement":null},{"id":"W2977372173","doi":"10.3847/1538-4357/ab8461","title":"Compact-object Mergers in the Galactic Center: Evolution in Triaxial Clusters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"University of Arizona","keywords":"Physics; Astrophysics; Supermassive black hole; Galactic Center; Star cluster; Galaxy; Milky Way; Astronomy; Gravitational wave; Velocity dispersion","score_opus":0.019497737460121112,"score_gpt":0.3126129324214042,"score_spread":0.2931151949612831,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2977372173","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99968576,0.000048598224,0.00004859229,0.00001100625,4.204109e-7,8.689917e-7,0.000026435731,0.0000032876196,0.0001749165],"genre_scores_gemma":[0.99982506,0.000027324257,0.000040070667,0.0000028720178,0.000001146191,7.1141136e-7,0.000060364786,0.000001721692,0.000040592953],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998869,0.00001711763,0.00000505645,0.000036167003,0.000020606374,0.00003424158],"domain_scores_gemma":[0.9992293,0.00009491264,0.00033287407,0.000054046333,0.0000715844,0.00021715755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022478128,0.00017604142,0.00018290873,0.0011297319,0.00061400124,0.00079942663,0.00029089904,0.00034383207,0.00093642913],"category_scores_gemma":[0.0008376158,0.0001303357,0.00016594319,0.00094975583,0.0005092499,0.0003705086,0.0008838729,0.00021055418,0.00021814261],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000347095,0.00007785569,0.96637374,0.00001540428,0.00007694585,0.00054896745,0.00049681234,0.006959005,0.020555953,0.0008983147,0.00022174857,0.0034281642],"study_design_scores_gemma":[0.000005942285,0.000051264433,0.98998636,0.0000027582903,0.000012384466,0.0004083144,0.0004247643,0.007554221,0.0011235449,0.00023121182,0.00018895758,0.000010310128],"about_ca_topic_score_codex":0.0045756795,"about_ca_topic_score_gemma":0.0041785617,"teacher_disagreement_score":0.0045756795,"about_ca_system_score_codex":0.0006011841,"about_ca_system_score_gemma":0.00019479642,"threshold_uncertainty_score":0.009098053},"labels":[],"label_agreement":null},{"id":"W2977534782","doi":"10.3847/1538-4357/ab53d9","title":"Chemical Abundances along the 1G Sequence of the Chromosome Maps: The Globular Cluster NGC 3201*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Globular cluster; Metallicity; Stars; Photometry (optics); Blue straggler; Main sequence; Population; Horizontal branch; Stellar population; Chemical evolution","score_opus":0.009605690797766728,"score_gpt":0.22038008433861778,"score_spread":0.21077439354085103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2977534782","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99921906,0.00003020983,0.000024017301,0.0000070674864,4.7127833e-7,0.0000013366243,0.00041514818,0.000004872621,0.00029782357],"genre_scores_gemma":[0.99836165,0.000022506736,0.00014423755,0.0000045398415,0.0000025986787,0.0000035864466,0.0010991779,0.0000024193766,0.0003592415],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992776,0.0000037724094,0.0000040543514,0.00003434394,0.000017431572,0.000012654579],"domain_scores_gemma":[0.9997193,0.000030108527,0.000111407026,0.000020648538,0.00004882391,0.00006958867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000064232074,0.00016038913,0.00012795144,0.0013462001,0.00031142205,0.00022222516,0.00012458254,0.0001678026,0.002128428],"category_scores_gemma":[0.00030328176,0.00005348455,0.000068583046,0.0006525114,0.00016370633,0.00010394377,0.00026392663,0.000080902115,0.0004215363],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023808285,0.00003123825,0.92363775,0.00003570366,0.000022437973,0.00016635102,0.00050522527,0.0005711578,0.06523003,0.00026769756,0.00041546294,0.008878877],"study_design_scores_gemma":[0.000002050336,0.000027304464,0.9983399,0.000001888833,0.00000387212,0.0000719372,0.0000624315,0.00023836635,0.00077249226,0.000036618163,0.0004416815,0.0000013370731],"about_ca_topic_score_codex":0.00413858,"about_ca_topic_score_gemma":0.0051336386,"teacher_disagreement_score":0.00413858,"about_ca_system_score_codex":0.00032787176,"about_ca_system_score_gemma":0.000103336286,"threshold_uncertainty_score":0.008229017},"labels":[],"label_agreement":null},{"id":"W2977800041","doi":"10.3847/1538-4357/ab3d36","title":"Disk–Jet Coupling in the 2017/2018 Outburst of the Galactic Black Hole Candidate X-Ray Binary MAXI J1535–571","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Labex UnivEarthS; Natural Sciences and Engineering Research Council of Canada; Government of Western Australia; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Curtin University of Technology; National Research Foundation; National Aeronautics and Space Administration; Agence Nationale de la Recherche; Commonwealth Scientific and Industrial Research Organisation; Australian Government","keywords":"Superluminal motion; Binary black hole; Black hole (networking); Proper motion; Binary number; Knot (papermaking); Jet (fluid); Active galactic nucleus","score_opus":0.013810807837900169,"score_gpt":0.237082265286739,"score_spread":0.22327145744883883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2977800041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994797,0.00006415809,0.00006594461,0.000014226054,0.000005087576,0.0000026758607,0.00007842147,0.000007804175,0.00028185177],"genre_scores_gemma":[0.9994777,0.000026792271,0.00007348336,0.000009222977,0.000007026782,0.0000027356666,0.00025158032,0.000003697952,0.00014782141],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999187,0.0000064825153,0.0000046449886,0.000028203189,0.000017081482,0.000024940835],"domain_scores_gemma":[0.99973077,0.000031966294,0.000113910384,0.000016710519,0.000027965114,0.000078658406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014326724,0.00016161375,0.00023209344,0.00044771237,0.0003642133,0.0005607538,0.00020021609,0.00021806048,0.00089875463],"category_scores_gemma":[0.00048845063,0.00011855634,0.00011449418,0.0002657905,0.00017805232,0.00020320306,0.0004993446,0.0002695989,0.00018142363],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006717328,0.0001256114,0.9338451,0.000040718845,0.00005258868,0.0041032513,0.0007662137,0.00039481418,0.046266433,0.0002516956,0.0005339302,0.012947868],"study_design_scores_gemma":[0.0000051379907,0.000055967932,0.9974112,0.000005987994,0.000011197217,0.0003644198,0.00016300692,0.00057527603,0.0009661635,0.000039268634,0.00039823644,0.0000041671897],"about_ca_topic_score_codex":0.003527732,"about_ca_topic_score_gemma":0.005450195,"teacher_disagreement_score":0.003527732,"about_ca_system_score_codex":0.00030268787,"about_ca_system_score_gemma":0.000112972295,"threshold_uncertainty_score":0.007014394},"labels":[],"label_agreement":null},{"id":"W2977800944","doi":"10.3847/1538-4357/ab498f","title":"The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. I. Identifying and Characterizing the Protostellar Content of the OMC-2 FIR4 and OMC-2 FIR3 Regions","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Protostar; Stars; Star formation; Outflow; Basso continuo; Emission spectrum; Accretion (finance); Accretion disc","score_opus":0.03215881490204261,"score_gpt":0.2524625151108229,"score_spread":0.2203037002087803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2977800944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987123,0.000056789802,0.000055591314,0.000016832177,0.0000013766987,0.000004512446,0.0004439764,0.000010229493,0.0006983337],"genre_scores_gemma":[0.99722004,0.000054432647,0.0005920747,0.000019962285,0.00000825783,0.000011013837,0.0015804784,0.0000057509033,0.0005079636],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987495,0.000012471971,0.0000072584608,0.00003543402,0.00003438007,0.000035491477],"domain_scores_gemma":[0.99960726,0.000028183222,0.00015391369,0.00003369917,0.000044290297,0.00013264078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017300042,0.00018303747,0.00015769408,0.0011445704,0.0004660235,0.00042416973,0.00030770202,0.0002121615,0.0008675866],"category_scores_gemma":[0.00037332927,0.00014537922,0.00015241142,0.00055620016,0.00019759436,0.00023741921,0.000577059,0.0001682382,0.00021021575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007156474,0.000029732928,0.9817555,0.000013704349,0.00002727115,0.00016765151,0.00029867253,0.000079905476,0.012604503,0.00007657863,0.000288426,0.0045865006],"study_design_scores_gemma":[0.000003502686,0.000011815458,0.9987733,0.0000026437065,0.0000049833748,0.000090970294,0.00009447585,0.00012045826,0.0002946212,0.000013600935,0.0005882452,0.0000013836774],"about_ca_topic_score_codex":0.012827184,"about_ca_topic_score_gemma":0.027442075,"teacher_disagreement_score":0.012827184,"about_ca_system_score_codex":0.0004954146,"about_ca_system_score_gemma":0.00021500456,"threshold_uncertainty_score":0.025505066},"labels":[],"label_agreement":null},{"id":"W2977903129","doi":"10.3847/1538-4357/ab40a8","title":"Improving the Epoch of Reionization Power Spectrum Results from Murchison Widefield Array Season 1 Observations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":138,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Reionization; Zenith; Epoch (astronomy); Spectral density; Wavelength; COSMIC cancer database; Dark Ages; Cosmology","score_opus":0.009441633676465333,"score_gpt":0.20138551177012953,"score_spread":0.1919438780936642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2977903129","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9770626,0.0003405947,0.015810905,0.00040196787,0.00005205327,0.000027995735,0.0019988113,0.00038595317,0.0039191693],"genre_scores_gemma":[0.9811111,0.00010188803,0.015773611,0.000088822395,0.00004151798,0.000017893106,0.0018292605,0.000110150744,0.000925857],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994967,0.00014225,0.000032981152,0.00012363977,0.00014866146,0.000055736884],"domain_scores_gemma":[0.99839634,0.0005218162,0.00027739207,0.00034772654,0.00037920804,0.00007753465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013483578,0.00033452376,0.00023674878,0.0005128065,0.00015077314,0.0005386339,0.00038531754,0.00030034507,0.0009910563],"category_scores_gemma":[0.0029527491,0.00017179434,0.0004374793,0.00045254442,0.00012328943,0.0005375709,0.00045151543,0.00027834845,0.00032974192],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040983333,0.000060237202,0.85404766,0.00013129413,0.0003577723,0.00014876384,0.000217823,0.02572465,0.061363243,0.001010121,0.0033225433,0.053206064],"study_design_scores_gemma":[0.00004616324,0.00006583144,0.9340034,0.000020728121,0.00014867594,0.000060323215,0.000054426022,0.045263287,0.015635287,0.00038977904,0.004276762,0.0000352865],"about_ca_topic_score_codex":0.00948513,"about_ca_topic_score_gemma":0.023261944,"teacher_disagreement_score":0.00948513,"about_ca_system_score_codex":0.0003471586,"about_ca_system_score_gemma":0.00024031433,"threshold_uncertainty_score":0.018859804},"labels":[],"label_agreement":null},{"id":"W2978091857","doi":"10.3847/1538-4357/ab48fb","title":"A Cepheid-based Distance to the Seyfert Galaxy NGC 6814","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Galaxy; Distance modulus; Hubble sequence; Logarithm; Cosmic distance ladder; Range (aeronautics)","score_opus":0.005276228052718199,"score_gpt":0.20341692268144038,"score_spread":0.1981406946287222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978091857","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944699,0.00012113521,0.00049586064,0.00002974372,0.0000043811697,0.000008870402,0.0013394846,0.000026422289,0.0035042411],"genre_scores_gemma":[0.9965982,0.000054714314,0.0010659915,0.0000070069054,0.0000072242487,0.000008545025,0.0017804486,0.000005909794,0.00047201585],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999782,0.000017933617,0.00001640967,0.000058538248,0.00008347382,0.00004161566],"domain_scores_gemma":[0.9990907,0.000087112305,0.0003460295,0.000072994284,0.00025188614,0.00015132113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017399664,0.00026138913,0.00022338209,0.0029910295,0.00043492,0.00056949194,0.0003147061,0.0002117335,0.0042357324],"category_scores_gemma":[0.0014526498,0.000102349804,0.00013054193,0.001245393,0.00022735813,0.00035476513,0.00088933867,0.00025071495,0.00069118704],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007428608,0.000025169837,0.97695017,0.000036953537,0.000057618832,0.00010054348,0.00019288603,0.00083428156,0.005575156,0.0006974483,0.0010832043,0.014372319],"study_design_scores_gemma":[0.0000034146983,0.000021893213,0.9970747,0.0000065207682,0.000007057877,0.00012149606,0.00008477505,0.0005426514,0.00039490423,0.0001558397,0.0015816127,0.000005188196],"about_ca_topic_score_codex":0.009939482,"about_ca_topic_score_gemma":0.018898064,"teacher_disagreement_score":0.009939482,"about_ca_system_score_codex":0.00042299205,"about_ca_system_score_gemma":0.00021682131,"threshold_uncertainty_score":0.01976329},"labels":[],"label_agreement":null},{"id":"W2978305136","doi":"10.3847/1538-4357/ab4adb","title":"A Search for Late-time Radio Emission and Fast Radio Bursts from Superluminous Supernovae","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; McGill University","funders":"","keywords":"Magnetar; Jansky; Supernova; Physics; Astrophysics; Neutron star; Pulsar; Ejecta; Luminosity; Astronomy; Light curve; Galaxy","score_opus":0.009178981989654838,"score_gpt":0.22528169770840964,"score_spread":0.2161027157187548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978305136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976914,0.00026841444,0.0010514203,0.00001967668,0.000004640755,0.000010849926,0.00028932767,0.000023714061,0.0006406162],"genre_scores_gemma":[0.9954823,0.00016764391,0.0024741078,0.000041553943,0.000013711951,0.000009244294,0.0014227349,0.000010926659,0.0003777817],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998242,0.000019190744,0.000012670259,0.00005629108,0.000039891616,0.000047787787],"domain_scores_gemma":[0.9990294,0.00019424211,0.00030140835,0.00009100759,0.000089477704,0.0002945445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046985596,0.00047604626,0.0003352456,0.0013541933,0.00029633657,0.00059910514,0.00035477625,0.00027695656,0.0011004726],"category_scores_gemma":[0.00049694034,0.00020492716,0.00046700984,0.0006818469,0.00021259689,0.00019949426,0.00047749595,0.00023568461,0.00031224173],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035342242,0.000098262586,0.84028506,0.000057960224,0.0001684807,0.0006695985,0.00013584053,0.0005447887,0.14022952,0.00022469183,0.000251951,0.016980374],"study_design_scores_gemma":[0.000019155554,0.00020349651,0.98576015,0.000007936103,0.000076898636,0.000960243,0.00010731042,0.0010256334,0.010565847,0.00013817051,0.0011228594,0.000012434931],"about_ca_topic_score_codex":0.0009963129,"about_ca_topic_score_gemma":0.0022560884,"teacher_disagreement_score":0.0013541933,"about_ca_system_score_codex":0.0001876952,"about_ca_system_score_gemma":0.00016964758,"threshold_uncertainty_score":0.003681481},"labels":[],"label_agreement":null},{"id":"W2978427143","doi":"10.3847/1538-4357/ab4b4a","title":"Tracing Magnetic Fields By the Synergies of Synchrotron Emission Gradients","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Natural Science Foundation of China","keywords":"Synchrotron; Magnetic field; Polarization (electrochemistry); Faraday effect; Synchrotron radiation; Galactic plane; Magnetohydrodynamics","score_opus":0.0041161879256724765,"score_gpt":0.20097433726122238,"score_spread":0.1968581493355499,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978427143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9034687,0.00017492611,0.09442289,0.000109439454,0.000010668567,0.000015507521,0.00010136834,0.00024590176,0.0014506172],"genre_scores_gemma":[0.98189145,0.000036125966,0.017920708,0.000007087222,0.00000298461,0.000003185107,0.000030845407,0.000010510348,0.00009712694],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999113,0.000029519457,0.0000035924043,0.000018409453,0.000024937748,0.000012225367],"domain_scores_gemma":[0.99969447,0.00013499161,0.00007385497,0.000031906537,0.0000354083,0.000029372044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032574532,0.00021502814,0.00017708234,0.00065320206,0.00013990089,0.00045462977,0.0002898777,0.00017661457,0.00036938163],"category_scores_gemma":[0.0014520654,0.00020324455,0.00021848317,0.0003554925,0.0003680333,0.0005271658,0.0005033027,0.0002206129,0.00005855451],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031044093,0.00011268867,0.11990394,0.00007774624,0.000111022564,0.00018331602,0.0002657811,0.7631147,0.05035306,0.009622126,0.00034651798,0.05559869],"study_design_scores_gemma":[0.0000118797325,0.000031197218,0.009223566,0.000005326176,0.000007737075,0.000045144276,0.000037528138,0.9846257,0.003992054,0.001680389,0.00032739225,0.000012049471],"about_ca_topic_score_codex":0.0031768808,"about_ca_topic_score_gemma":0.004069656,"teacher_disagreement_score":0.0031768808,"about_ca_system_score_codex":0.00029138618,"about_ca_system_score_gemma":0.000298233,"threshold_uncertainty_score":0.006316781},"labels":[],"label_agreement":null},{"id":"W2978646844","doi":"10.3847/1538-4357/ab65f8","title":"Analysis of Multi-hour Continuous Observations of Seven Millisecond Pulsars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Pulsar; Millisecond pulsar; Scintillation; Millisecond; Gravitational wave; Radio telescope; Noise (video); Pulse (music); Neutron star","score_opus":0.03484716588783021,"score_gpt":0.3190108290575673,"score_spread":0.28416366316973707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2978646844","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986676,0.000043537977,0.00074998836,0.0000099634,0.000004272669,0.000004122535,0.0002634279,0.000017465694,0.00023961949],"genre_scores_gemma":[0.99814343,0.000021459062,0.00065371435,0.000005372686,0.000016705371,0.0000067090273,0.0010442282,0.000009360136,0.00009898043],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99946016,0.000059490794,0.000041467432,0.000110308596,0.00025894886,0.00006969427],"domain_scores_gemma":[0.9971175,0.00097375584,0.00086806255,0.0003300033,0.00045296075,0.00025762327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00092068064,0.00019015241,0.00033087967,0.0014995678,0.00029165996,0.00042307476,0.00038977998,0.0002541477,0.00046121902],"category_scores_gemma":[0.0026777338,0.00014763844,0.00023487073,0.0012553157,0.00022572711,0.00022039507,0.00063950033,0.0003207707,0.00011930413],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005978422,0.00009971613,0.92062086,0.00006630925,0.0002578133,0.00040177745,0.0005236779,0.0021207326,0.045174845,0.00024995964,0.0003108531,0.029575517],"study_design_scores_gemma":[0.0000043292353,0.00005401652,0.99671906,0.0000022691002,0.00001876736,0.00010575639,0.00003984984,0.0014255107,0.0012974442,0.000031259595,0.00029717846,0.0000045444604],"about_ca_topic_score_codex":0.0019237313,"about_ca_topic_score_gemma":0.0028129136,"teacher_disagreement_score":0.0019237313,"about_ca_system_score_codex":0.00020483321,"about_ca_system_score_gemma":0.00013779357,"threshold_uncertainty_score":0.0048691034},"labels":[],"label_agreement":null},{"id":"W2979088950","doi":"10.3847/1538-4357/ab8f24","title":"A Measurement of the Degree-scale CMB B-mode Angular Power Spectrum with Polarbear","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":71,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Advanced Research; Dalhousie University","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Labex UnivEarthS; Comisión Nacional de Investigación Científica y Tecnológica; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of California, San Diego; University of Melbourne; Office of Science; Ministry of Education, Culture, Sports, Science and Technology; Agence Nationale de la Recherche; U.S. Department of Energy; European Commission; National Energy Research Scientific Computing Center; John Templeton Foundation; Gordon and Betty Moore Foundation; Simons Foundation; National Science Foundation","keywords":"Physics; Cosmic microwave background; Spectral density; Planck; Polarization (electrochemistry); Astrophysics; Spectral line; Spectral index; Lambda; Cosmic background radiation; Anisotropy; Optics; Quantum mechanics; Statistics","score_opus":0.013487323167542762,"score_gpt":0.2186111164830138,"score_spread":0.20512379331547104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979088950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.962139,0.00031594708,0.01742181,0.00019845554,0.000044461423,0.000024310537,0.00713939,0.00048150978,0.012235105],"genre_scores_gemma":[0.99018127,0.00011625379,0.005373683,0.000067709036,0.00004350828,0.000021411675,0.0035279253,0.00007105238,0.0005970298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977833,0.000044164113,0.000007708814,0.000078498335,0.000067878886,0.000023336685],"domain_scores_gemma":[0.99954563,0.00012316236,0.00010613907,0.000079306024,0.00009301127,0.00005259805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031516273,0.0003152592,0.00014559356,0.0014116123,0.00020286856,0.0005026035,0.00018438805,0.00021381721,0.0024237193],"category_scores_gemma":[0.0008156718,0.00018545354,0.00012579706,0.0009359679,0.00020491076,0.00038665772,0.00037601992,0.0003308522,0.0007036723],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008208489,0.00015865106,0.7268732,0.00013538294,0.00029896927,0.0003396536,0.0002822149,0.005287827,0.1983118,0.0029554693,0.0062383567,0.058297604],"study_design_scores_gemma":[0.000021840477,0.00008947151,0.9392663,0.000023683093,0.000051771472,0.0003833136,0.00008930443,0.008038027,0.04365442,0.0011286786,0.0072201025,0.000033007997],"about_ca_topic_score_codex":0.0008533079,"about_ca_topic_score_gemma":0.001250768,"teacher_disagreement_score":0.0024237193,"about_ca_system_score_codex":0.00013072904,"about_ca_system_score_gemma":0.000054274926,"threshold_uncertainty_score":0.008108199},"labels":[],"label_agreement":null},{"id":"W2979333579","doi":"10.3847/1538-4357/ab9b25","title":"The Dragonfly Edge-on Galaxies Survey: Shaping the Outer disk of NGC 4565 via Accretion","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Starlight; Surface brightness; Galaxy; Accretion (finance); Asymmetry; Hubble sequence; Sky; Extinction (optical mineralogy)","score_opus":0.019437131974509744,"score_gpt":0.22922301608417345,"score_spread":0.2097858841096637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979333579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99911267,0.000059531223,0.00013006474,0.000011196408,0.0000012639615,0.0000018333969,0.00011868941,0.000011845302,0.00055275223],"genre_scores_gemma":[0.99963474,0.000018926152,0.00013176615,0.000010927261,0.0000013927516,6.7277546e-7,0.00012178837,0.000001693769,0.00007809001],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998908,0.000012689822,0.0000052563128,0.000034598885,0.000019391271,0.00003722114],"domain_scores_gemma":[0.9997354,0.000021482792,0.00008222664,0.000032123706,0.000021814047,0.0001068868],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019894283,0.00023179292,0.00015270323,0.0010594497,0.00030775394,0.00059511914,0.00020634376,0.00015660546,0.0005295923],"category_scores_gemma":[0.00026524748,0.00012027769,0.00015207319,0.0004457998,0.00034422663,0.00020187444,0.00051921455,0.00011274199,0.00010753204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012742239,0.000029678838,0.9556868,0.000024117451,0.000059541057,0.00034432125,0.00072280766,0.00035537264,0.03388139,0.00029570647,0.00033076585,0.008142144],"study_design_scores_gemma":[0.000002415321,0.000019317546,0.99785405,0.000005017761,0.000012464356,0.000115474664,0.00023168825,0.0002749244,0.0009362257,0.00003965488,0.0005052175,0.000003492954],"about_ca_topic_score_codex":0.016560528,"about_ca_topic_score_gemma":0.035692662,"teacher_disagreement_score":0.016560528,"about_ca_system_score_codex":0.00044690777,"about_ca_system_score_gemma":0.00012678551,"threshold_uncertainty_score":0.032928288},"labels":[],"label_agreement":null},{"id":"W2979492295","doi":"10.3847/1538-4357/ab4a77","title":"Dwarfs or Giants? Stellar Metallicities and Distances from ugrizG Multiband Photometry","year":2019,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Photometry (optics); Astrophysics; Stars; Metallicity; Halo; Galaxy; Dwarf galaxy; Astronomy","score_opus":0.017794724641334546,"score_gpt":0.24557308236132733,"score_spread":0.22777835771999277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979492295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95878136,0.0005896707,0.029115697,0.00031414657,0.000027195481,0.00003570213,0.004015312,0.0024951005,0.0046258424],"genre_scores_gemma":[0.9619631,0.00008035385,0.03139645,0.00006415018,0.000017499311,0.000013026377,0.0049714926,0.00012672313,0.0013671481],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997584,0.000032443935,0.000012903977,0.00010317183,0.000055472985,0.000037703845],"domain_scores_gemma":[0.99953675,0.00009817792,0.000079061705,0.000100041776,0.00013283166,0.0000530178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047714153,0.00033047897,0.00030999753,0.0011664352,0.00019081644,0.0010090917,0.00043189782,0.00038899708,0.0014381545],"category_scores_gemma":[0.0021416997,0.00010850076,0.00017762791,0.0005307525,0.0002062106,0.00031564597,0.00050842273,0.00018808038,0.0015768199],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027680356,0.00004034516,0.75607026,0.00006237088,0.00012799517,0.00006470434,0.0002297414,0.01642439,0.013368474,0.00091421825,0.008902733,0.20351788],"study_design_scores_gemma":[0.000037524558,0.000050174633,0.7189764,0.00004932397,0.000050443603,0.00014019985,0.0003111468,0.2547778,0.012739182,0.0018527802,0.0109834075,0.000031671312],"about_ca_topic_score_codex":0.012380542,"about_ca_topic_score_gemma":0.01592959,"teacher_disagreement_score":0.012380542,"about_ca_system_score_codex":0.0005450272,"about_ca_system_score_gemma":0.00025602206,"threshold_uncertainty_score":0.024616957},"labels":[],"label_agreement":null},{"id":"W2979513896","doi":"10.3847/1538-4357/ab4d53","title":"Multi-wavelength Properties of Radio- and Machine-learning-identified Counterparts to Submillimeter Sources in S2COSMOS","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; McMaster University; Dalhousie University","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Redshift; Population; Submillimeter Array; Confusion; Star formation; Source counts; Photometric redshift; Stellar mass","score_opus":0.011765979373505242,"score_gpt":0.19920331107120035,"score_spread":0.1874373316976951,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979513896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986039,0.000060705424,0.00026362872,0.000014719056,0.0000033363954,0.000004431224,0.0004995062,0.000030943735,0.00051880424],"genre_scores_gemma":[0.9958366,0.000053469514,0.0005737845,0.000022876708,0.000019253688,0.000011446467,0.0030794784,0.00002407131,0.00037908045],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998166,0.000015669826,0.000013910594,0.0000720535,0.000043529126,0.0000382108],"domain_scores_gemma":[0.99867827,0.00017253535,0.0005430964,0.0001686135,0.00020631749,0.00023110583],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004440558,0.00031912568,0.00024746044,0.0018471911,0.00027170894,0.0005739185,0.0003386445,0.0002121868,0.0017793399],"category_scores_gemma":[0.001119067,0.00016665547,0.00027525917,0.0012460182,0.00018856664,0.0003648418,0.00067809125,0.00021180375,0.0006423784],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009340239,0.00004269936,0.981556,0.000025578373,0.000063862404,0.00019477222,0.00024490655,0.0009791767,0.00851017,0.00018959954,0.00067376374,0.0074261255],"study_design_scores_gemma":[0.0000063200814,0.000014965519,0.9965019,0.0000061394358,0.000013360194,0.00008682728,0.000059914164,0.002173467,0.0005986708,0.000057262987,0.0004771156,0.000004132957],"about_ca_topic_score_codex":0.0031615007,"about_ca_topic_score_gemma":0.0055488907,"teacher_disagreement_score":0.0031615007,"about_ca_system_score_codex":0.00023152963,"about_ca_system_score_gemma":0.00013329653,"threshold_uncertainty_score":0.006286204},"labels":[],"label_agreement":null},{"id":"W2979556488","doi":"10.3847/1538-4357/ab40cb","title":"Supermassive Black Hole Binary Candidates from the Pan-STARRS1 Medium Deep Survey","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":98,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Office of Science; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Max-Planck-Gesellschaft; Lawrence Berkeley National Laboratory; Ministerio de Ciencia, Tecnología e Innovación Productiva; Durham University; York University; Space Telescope Science Institute; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Brookhaven National Laboratory; Ministério da Ciência, Tecnologia e Inovação; Northern Arizona University; Harvard University; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University","keywords":"Physics; Quasar; Supermassive black hole; Astrophysics; Binary black hole; Sky; Observatory; Blazar; Binary number; Telescope; Astronomy; Galaxy; Gravitational wave; Gamma ray","score_opus":0.007503226125853624,"score_gpt":0.20762144643492442,"score_spread":0.20011822030907078,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979556488","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989207,0.00007392375,0.00013561563,0.000017359711,0.0000010379414,0.0000060002194,0.00048816603,0.000010756535,0.00034654257],"genre_scores_gemma":[0.9983374,0.000047763846,0.0003044883,0.000009281803,0.0000041213134,0.000005121599,0.0011064607,0.0000029129883,0.0001822785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977034,0.000037738933,0.000015548188,0.00006859423,0.00006358897,0.000044232977],"domain_scores_gemma":[0.9988967,0.00015885902,0.0004429874,0.00014050178,0.00011289227,0.00024799528],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057664333,0.00016597801,0.00019331748,0.0018342999,0.0003049844,0.0003977921,0.00029482724,0.0001269245,0.0012045985],"category_scores_gemma":[0.0012772657,0.000120292374,0.0001603347,0.0005923516,0.0001873637,0.00025366037,0.00087154214,0.00014360124,0.00022806266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005541579,0.000012653706,0.98933125,0.0000146144985,0.000025851941,0.00009649406,0.00009294135,0.000087514054,0.0043433825,0.00006417472,0.00022801828,0.005647666],"study_design_scores_gemma":[0.000003061719,0.000027608212,0.99841356,0.0000036344181,0.0000119546685,0.00021572229,0.00008656746,0.00021518047,0.00045690255,0.000020025765,0.00054362393,0.0000022407748],"about_ca_topic_score_codex":0.00298068,"about_ca_topic_score_gemma":0.011887462,"teacher_disagreement_score":0.00298068,"about_ca_system_score_codex":0.00016566808,"about_ca_system_score_gemma":0.00019066314,"threshold_uncertainty_score":0.0059266686},"labels":[],"label_agreement":null},{"id":"W2979560498","doi":"10.3847/1538-4357/ab290d","title":"Spatially Resolved Water Emission from Gravitationally Lensed Dusty Star-forming Galaxies at z ∼ 3","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Dalhousie University","funders":"National Astronomical Observatory of Japan; Gordon and Betty Moore Foundation; Alfred P. Sloan Foundation; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Galaxy; Redshift; Active galactic nucleus; Luminosity; Luminous infrared galaxy; Star formation; Emission spectrum; Radio galaxy","score_opus":0.009737893352043057,"score_gpt":0.22311016899132594,"score_spread":0.21337227563928288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979560498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99949026,0.000029281644,0.00010878994,0.0000077226905,7.7320453e-7,0.0000016111832,0.00015566505,0.000010894614,0.00019489872],"genre_scores_gemma":[0.9994686,0.000011938792,0.00017537102,0.0000087221615,0.000002922489,0.0000013012162,0.0002243605,0.0000020902646,0.000104569524],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989927,0.000011580192,0.000004718198,0.000037396505,0.000018835877,0.000028198068],"domain_scores_gemma":[0.9996196,0.000051068713,0.00012313448,0.000039317278,0.000032294447,0.00013456173],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019418,0.000174766,0.000188649,0.00073762715,0.00027584162,0.00036825772,0.00028465036,0.00021545192,0.0010238844],"category_scores_gemma":[0.00021686907,0.00018140132,0.00018902747,0.0004511601,0.00027075963,0.00019083082,0.00039988174,0.00019785397,0.00015723733],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027814566,0.00009049507,0.9197876,0.00002106982,0.00009223303,0.0001979669,0.00042624294,0.00027551013,0.0732727,0.00013002093,0.00021400061,0.005214122],"study_design_scores_gemma":[0.0000040379177,0.000024081577,0.99856704,0.0000010024645,0.000008282385,0.000044488046,0.000055400276,0.00019906486,0.0009879682,0.00001783345,0.000089282636,0.0000015717948],"about_ca_topic_score_codex":0.004930519,"about_ca_topic_score_gemma":0.009159607,"teacher_disagreement_score":0.004930519,"about_ca_system_score_codex":0.00025880072,"about_ca_system_score_gemma":0.00007228287,"threshold_uncertainty_score":0.009803653},"labels":[],"label_agreement":null},{"id":"W2979810526","doi":"10.3847/1538-4357/ab50c3","title":"ROBO-AO Kepler Asteroseismic Survey. II. Do Stellar Companions Inhibit Stellar Oscillations?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Aeronautics and Space Administration","keywords":"Stars; Oscillation (cell signaling); Amplitude; Asteroseismology; Photometry (optics); Telescope; Spitzer Space Telescope","score_opus":0.028508384290213577,"score_gpt":0.23772487628929007,"score_spread":0.2092164919990765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979810526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99791676,0.00030983475,0.00004735149,0.000023076658,0.0000020496411,0.0000030029871,0.00035586342,0.0000037141435,0.0013384548],"genre_scores_gemma":[0.99879515,0.00012497087,0.000081248945,0.000013036491,0.0000046789205,0.000002275612,0.0006802092,0.000002803774,0.00029562344],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997472,0.000040836847,0.000024545176,0.00006613081,0.0000626056,0.000058675098],"domain_scores_gemma":[0.9984205,0.00022408311,0.0007467425,0.00012045889,0.00020016576,0.0002880271],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044714467,0.00015749001,0.00026802375,0.00069858244,0.00032574905,0.00047144125,0.00023993356,0.00019188486,0.0011055741],"category_scores_gemma":[0.0013726988,0.000110041605,0.00010634457,0.00044742398,0.00022784292,0.00029202917,0.00040298083,0.00014462954,0.00047362965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018055107,0.000032792355,0.98912525,0.00002933383,0.000026474536,0.00010409192,0.00010740087,0.000029100862,0.0053995354,0.00008351403,0.0001636912,0.0047183186],"study_design_scores_gemma":[0.0000039890565,0.000028668555,0.9985549,0.0000027693459,0.000009845799,0.00016663008,0.00008570727,0.000073705036,0.0003868071,0.000018020386,0.0006679521,9.598365e-7],"about_ca_topic_score_codex":0.0057224873,"about_ca_topic_score_gemma":0.008964482,"teacher_disagreement_score":0.0057224873,"about_ca_system_score_codex":0.00019591907,"about_ca_system_score_gemma":0.00016846374,"threshold_uncertainty_score":0.011378348},"labels":[],"label_agreement":null},{"id":"W2979899281","doi":"10.3847/1538-4357/ab4186","title":"A Measurement of the Cosmic Microwave Background Lensing Potential and Power Spectrum from 500 deg<sup>2</sup> of SPTpol Temperature and Polarization Data","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Three-Speed Logic (Canada); Canadian Institute for Advanced Research; McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of Colorado Boulder; Office of Science; Argonne National Laboratory; National Energy Research Scientific Computing Center; McGill University; Gordon and Betty Moore Foundation; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Physics; Cosmic microwave background; Analytical Chemistry (journal); Optics; Anisotropy; Chemistry","score_opus":0.00980463165603103,"score_gpt":0.21640621759762435,"score_spread":0.20660158594159334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2979899281","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989972,0.00005829259,0.0050820797,0.00007867087,0.000005316996,0.0000081973885,0.0022316626,0.00027468553,0.0022889497],"genre_scores_gemma":[0.9930184,0.000031317348,0.0030704224,0.000021017573,0.000014066973,0.00000848091,0.0035604464,0.00007255376,0.00020328537],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958533,0.00007244089,0.000016163423,0.00008079446,0.00019031252,0.000054893695],"domain_scores_gemma":[0.9988984,0.00040105387,0.00022567392,0.00019099818,0.00019663593,0.00008728213],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043560565,0.0003300426,0.00018111701,0.0009991952,0.0001961905,0.0004941909,0.00034969737,0.00026666443,0.0013681548],"category_scores_gemma":[0.0017343599,0.00024179948,0.00024121738,0.001198734,0.00021446955,0.00035690548,0.00023853169,0.0003186153,0.00043549918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013462816,0.00012247376,0.693345,0.00013501004,0.0004441137,0.0009250904,0.00036190214,0.022638677,0.21224263,0.002144325,0.004634263,0.061660156],"study_design_scores_gemma":[0.00002454235,0.00008088259,0.91698337,0.000010861467,0.00008122959,0.0003833346,0.00007695733,0.029073572,0.050251566,0.00036610724,0.002633363,0.000034256926],"about_ca_topic_score_codex":0.0025970493,"about_ca_topic_score_gemma":0.0052769994,"teacher_disagreement_score":0.0025970493,"about_ca_system_score_codex":0.00038725566,"about_ca_system_score_gemma":0.00012891158,"threshold_uncertainty_score":0.0051638484},"labels":[],"label_agreement":null},{"id":"W2980029064","doi":"10.3847/1538-4357/ab379c","title":"Cooling+Heating Flows in Galaxy Clusters: Turbulent Heating, Spectral Modeling, and Cooling Efficiency","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Perimeter Institute","funders":"","keywords":"Cooling flow; Physics; Intracluster medium; Radiative cooling; Astrophysics; Turbulence; Galaxy cluster; Magnetohydrodynamics; Spectral line; Magnetohydrodynamic drive; Galaxy; Computational physics; Mechanics; Plasma; Astronomy","score_opus":0.007815317038079915,"score_gpt":0.21710980676189934,"score_spread":0.20929448972381942,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980029064","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905128,0.00015399655,0.007459763,0.00007833194,0.0000062384843,0.000009699968,0.00006986015,0.000109428314,0.0016000064],"genre_scores_gemma":[0.99923897,0.00003618368,0.0005101152,0.000005548878,0.000004174257,0.0000032405208,0.000027826749,0.0000121997755,0.00016174975],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992454,0.000024975636,0.0000030488713,0.000019460138,0.000008832859,0.000019067626],"domain_scores_gemma":[0.9996093,0.0001277279,0.00010355149,0.000053407082,0.000042730513,0.00006330954],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004435591,0.00065472565,0.00026238937,0.0004898095,0.00038988938,0.0008188518,0.0006802778,0.00042256204,0.0005845028],"category_scores_gemma":[0.0012536736,0.00020465517,0.00028817807,0.00044225348,0.0007825516,0.00046521376,0.00044735658,0.00021279116,0.00015651199],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008272208,0.0000305673,0.047674634,0.00001964728,0.000034641347,0.00006168901,0.00008787021,0.94175833,0.002710969,0.0056778365,0.0002768013,0.0015843366],"study_design_scores_gemma":[0.000010579055,0.000011594279,0.012170364,0.0000031042803,0.0000067461096,0.000009729955,0.00001813134,0.98576397,0.0004654485,0.0014033789,0.00012917595,0.000007741183],"about_ca_topic_score_codex":0.025485503,"about_ca_topic_score_gemma":0.0069331536,"teacher_disagreement_score":0.025485503,"about_ca_system_score_codex":0.00085291604,"about_ca_system_score_gemma":0.00034214533,"threshold_uncertainty_score":0.05067432},"labels":[],"label_agreement":null},{"id":"W2980220644","doi":"10.3847/1538-4357/ab32eb","title":"Hunting for the Dark Matter Wake Induced by the Large Magellanic Cloud","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":198,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Dark matter; Halo; Galaxy; Astronomy; Milky Way; Large Magellanic Cloud; Dark matter halo; Local Group; Galactic halo; Satellite galaxy; Redshift; Stars","score_opus":0.006796474629283419,"score_gpt":0.21292980238076378,"score_spread":0.20613332775148036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980220644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955354,0.000048505277,0.0016284579,0.00016801922,0.000022584407,0.0000113572905,0.00006739148,0.00004389959,0.0024743662],"genre_scores_gemma":[0.99910957,0.000014588917,0.00048966147,0.00003423138,0.000007239173,0.000006022292,0.0000526072,0.00000962701,0.00027644628],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999232,0.000016084345,0.0000021631174,0.000009988532,0.0000112744265,0.000037181082],"domain_scores_gemma":[0.99965703,0.000095018215,0.000056438825,0.00002549092,0.000022176102,0.00014382474],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028120843,0.0002467899,0.0003912848,0.00021342431,0.0007483028,0.0007458207,0.0006292894,0.00067210523,0.0016997302],"category_scores_gemma":[0.0009533065,0.00020047704,0.00055376027,0.00014414133,0.0007580677,0.00048030826,0.0008415643,0.00066024106,0.00011446264],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002664445,0.00020891202,0.05735009,0.000041397514,0.00016476556,0.0006230314,0.00022801076,0.9265476,0.006743843,0.004105333,0.0012661455,0.0024545575],"study_design_scores_gemma":[0.00006476617,0.000076861514,0.012849032,0.0000072025928,0.000019462994,0.000032721982,0.0001032817,0.9849893,0.00048590894,0.001012769,0.00034606867,0.000012746869],"about_ca_topic_score_codex":0.022071494,"about_ca_topic_score_gemma":0.014982476,"teacher_disagreement_score":0.022071494,"about_ca_system_score_codex":0.0005927238,"about_ca_system_score_gemma":0.00066133967,"threshold_uncertainty_score":0.043886006},"labels":[],"label_agreement":null},{"id":"W2980354272","doi":"10.3847/1538-4357/ab480e","title":"Measurements of Low Temperature Rate Coefficients for the Reaction of CH with CH<sub>2</sub>O and Application to Dark Cloud and AGB Stellar Wind Models","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council; Vlaamse regering; Fonds Wetenschappelijk Onderzoek; University of Leeds","keywords":"Outflow; Photodissociation; Molecular cloud; Luminosity; Range (aeronautics); Asymptotic giant branch; Interstellar cloud; Nozzle; Collision","score_opus":0.009759544020264055,"score_gpt":0.21996517811974456,"score_spread":0.2102056340994805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980354272","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959359,0.00008681463,0.0031718896,0.000010646376,0.0000025494248,0.000018783936,0.0003128576,0.00007060787,0.00038999115],"genre_scores_gemma":[0.9989838,0.00003102177,0.00073555345,0.000001701967,8.7647356e-7,0.000006858561,0.0001584944,0.00000823514,0.00007348446],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985313,0.000017305385,0.0000063807,0.000049734503,0.00004739774,0.000025882806],"domain_scores_gemma":[0.9994518,0.00026562216,0.000115219635,0.000056319343,0.00007006156,0.000040997937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005117569,0.00048274203,0.00021072365,0.0005451992,0.00021910275,0.0002838068,0.00056203635,0.0004349714,0.0006934819],"category_scores_gemma":[0.0009451488,0.00030807656,0.000296338,0.0002552397,0.0003558319,0.000290947,0.00022536324,0.0004033881,0.00017443219],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077308476,0.00014184864,0.1399447,0.00010894307,0.000089300265,0.0001678636,0.00018288221,0.030620715,0.82164794,0.00076576247,0.00014254976,0.0054143104],"study_design_scores_gemma":[0.00006607786,0.00029903633,0.14120595,0.000008333447,0.00004077836,0.00018140618,0.00006199578,0.15357922,0.7037362,0.00026176733,0.000510023,0.000049172195],"about_ca_topic_score_codex":0.0036645369,"about_ca_topic_score_gemma":0.0027439883,"teacher_disagreement_score":0.0036645369,"about_ca_system_score_codex":0.0007564437,"about_ca_system_score_gemma":0.000135751,"threshold_uncertainty_score":0.00728637},"labels":[],"label_agreement":null},{"id":"W2980445246","doi":"10.3847/1538-4357/ab7b6e","title":"A 3D Radiation Hydrodynamic AGB Binary Model","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Compute Canada; Canadian Institute for Theoretical Astrophysics","keywords":"Circumbinary planet; Binary number; Accretion (finance); Binary star; Outflow; Stars; Mass transfer; Radiative transfer; Angular momentum","score_opus":0.011206172733469149,"score_gpt":0.2268745539439021,"score_spread":0.21566838121043294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980445246","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86334217,0.00086720596,0.067083456,0.0017413971,0.00024062638,0.00019188617,0.0033735528,0.0005461435,0.062613636],"genre_scores_gemma":[0.9786928,0.00024881776,0.010466379,0.00022613844,0.00006151387,0.00023156674,0.00084526796,0.000064943786,0.009162671],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985313,0.000047711575,0.0000067940728,0.000029827426,0.000031313062,0.000031206277],"domain_scores_gemma":[0.999694,0.0000671985,0.000058149908,0.000026823152,0.00006596523,0.00008782954],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021852461,0.000672557,0.00097592914,0.00059267523,0.001177312,0.0014379532,0.0015933028,0.0022223387,0.0063417032],"category_scores_gemma":[0.00069049996,0.0006090466,0.0008422354,0.0006813568,0.0010859945,0.00067652913,0.0014749517,0.0009063943,0.0007056695],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011275244,0.00006666417,0.0029509393,0.000042832216,0.000042401043,0.00029783385,0.000064500404,0.9817156,0.0012507553,0.011373989,0.00060836494,0.0014732467],"study_design_scores_gemma":[0.000048617938,0.000015729462,0.0004476975,0.000004966729,0.000006774306,0.000023081662,0.000022178163,0.9977563,0.00007659252,0.0011225169,0.0004684229,0.000007119548],"about_ca_topic_score_codex":0.034441806,"about_ca_topic_score_gemma":0.00941118,"teacher_disagreement_score":0.034441806,"about_ca_system_score_codex":0.0013261309,"about_ca_system_score_gemma":0.0010027832,"threshold_uncertainty_score":0.06848264},"labels":[],"label_agreement":null},{"id":"W2980489856","doi":"10.3847/1538-4357/ab4f85","title":"Eight Millisecond Pulsars Discovered in the Arecibo PALFA Survey","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia; McGill University","funders":"Precursory Research for Embryonic Science and Technology; Science and Technology Facilities Council; National Research Council Canada; Natural Sciences and Engineering Research Council of Canada; State Key Laboratory of Automotive Simulation and Control; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Natural Science Foundation of China; National Science Foundation; Compute Canada; Canarie; McGill University; Chinese Academy of Sciences; Canadian Institute for Advanced Research; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Millisecond pulsar; Pulsar; Physics; Astrophysics; Astronomy; Galactic plane; White dwarf; Binary pulsar; Population; Orbital period; Galaxy; Stars","score_opus":0.014429359904106228,"score_gpt":0.30339171288854616,"score_spread":0.28896235298443995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980489856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99595535,0.00042944358,0.00016227982,0.00005621702,0.000009317235,0.0000140771135,0.0006602616,0.000023095965,0.0026899779],"genre_scores_gemma":[0.9960303,0.00047600258,0.00051458116,0.00005836815,0.00002175342,0.000022899801,0.0019784379,0.000009272664,0.0008884625],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981564,0.000018464201,0.000007768527,0.000046343936,0.000048012724,0.00006375215],"domain_scores_gemma":[0.9995357,0.00005195793,0.00017872051,0.000039654788,0.00010661512,0.00008740289],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029044622,0.0002380775,0.00021438205,0.0018129288,0.0005660032,0.00050712103,0.00030972602,0.00020676029,0.0011754973],"category_scores_gemma":[0.0005464191,0.00012838408,0.00011324788,0.0014354733,0.00024155986,0.0002573794,0.00069807435,0.00022290614,0.00028993963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015650531,0.00003738716,0.9697789,0.000037468755,0.000027362785,0.000229464,0.00054111244,0.000030915748,0.006689779,0.00013313086,0.0008587094,0.021479256],"study_design_scores_gemma":[0.0000048668394,0.000022367529,0.99594927,0.0000063391403,0.00000786269,0.00017750818,0.00018456152,0.00003687265,0.00026109559,0.000017465962,0.0033298803,0.0000018019745],"about_ca_topic_score_codex":0.016461404,"about_ca_topic_score_gemma":0.027578473,"teacher_disagreement_score":0.016461404,"about_ca_system_score_codex":0.0005144662,"about_ca_system_score_gemma":0.0003329374,"threshold_uncertainty_score":0.032731175},"labels":[],"label_agreement":null},{"id":"W2980508536","doi":"10.3847/1538-4357/ab41fb","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Comparison of Lag Measurement Methods with Simulated Observations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Reverberation mapping; Light curve; Lag; Noise (video); Mathematics; Statistics; Physics; Computer science; Quasar; Astrophysics; Artificial intelligence","score_opus":0.06807847599108223,"score_gpt":0.3098031401226691,"score_spread":0.24172466413158683,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980508536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96299225,0.00017634267,0.033674903,0.00008476359,0.000016684064,0.00006399511,0.0009889969,0.0011052067,0.0008968663],"genre_scores_gemma":[0.9643098,0.00005597248,0.03298338,0.000030019139,0.000008781918,0.00006193155,0.0022025513,0.00015491075,0.00019274047],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9970258,0.0018935555,0.00013884413,0.00040006865,0.00042378376,0.00011792316],"domain_scores_gemma":[0.9790202,0.012702222,0.002051562,0.0035378211,0.0022805277,0.00040773675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.010646276,0.00052505184,0.0003468458,0.0010641047,0.0003767088,0.0008734468,0.0010015382,0.00056221965,0.0004895285],"category_scores_gemma":[0.027758427,0.00031084512,0.00038337146,0.0011313747,0.00032335878,0.00078141486,0.00084992894,0.0003933884,0.00019134516],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023307651,0.00051482755,0.38033918,0.0002546157,0.0005606123,0.00018150563,0.0005611032,0.49424845,0.004447118,0.0027223667,0.0029162017,0.110923335],"study_design_scores_gemma":[0.00017089264,0.00033400205,0.09842889,0.000038033355,0.00003852736,0.00013676757,0.00014338439,0.8931659,0.0056669856,0.0007241179,0.0010975449,0.000055024768],"about_ca_topic_score_codex":0.018325156,"about_ca_topic_score_gemma":0.015664788,"teacher_disagreement_score":0.018325156,"about_ca_system_score_codex":0.00088942895,"about_ca_system_score_gemma":0.0008813323,"threshold_uncertainty_score":0.0563035},"labels":[],"label_agreement":null},{"id":"W2980667535","doi":"10.3847/1538-4357/ab5115","title":"Mapping Metallicity Variations across Nearby Galaxy Disks","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":166,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Australian Research Council; European Commission; Natural Sciences and Engineering Research Council of Canada; Centre National d’Etudes Spatiales; Deutsche Forschungsgemeinschaft; Centre National de la Recherche Scientifique","keywords":"Metallicity; Galaxy; Spiral galaxy; Star formation; Interstellar medium; Spectroscopy; Irregular galaxy; Baryon","score_opus":0.010215649699383891,"score_gpt":0.23370166037036405,"score_spread":0.22348601067098017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2980667535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99934715,0.000033401797,0.000098556455,0.000004093916,4.3003965e-7,0.0000015834834,0.00026729223,0.000009361974,0.00023801911],"genre_scores_gemma":[0.99914837,0.000017022387,0.0002361095,0.000004147848,0.0000013691083,0.0000020480843,0.00047923837,0.000002943504,0.00010874786],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984145,0.000023166522,0.000008927113,0.00006694192,0.000031621184,0.000027924925],"domain_scores_gemma":[0.9994849,0.000071492235,0.0001744476,0.00007593142,0.000096402066,0.000096843265],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021509171,0.00015416597,0.00018693222,0.0014826603,0.00022570688,0.00037078283,0.00023373235,0.0001693862,0.00072236016],"category_scores_gemma":[0.0006355912,0.00011384729,0.00011895652,0.0008606796,0.00016655779,0.00019935737,0.00039105077,0.00008684628,0.00027024254],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049614002,0.000008815225,0.9856786,0.000008339897,0.00003030348,0.0000333441,0.00015230014,0.00016634061,0.009201243,0.00002380583,0.000064715576,0.004582589],"study_design_scores_gemma":[9.174577e-7,0.00001258201,0.99910563,0.0000013609749,0.00000428482,0.000031002037,0.00008696992,0.00018204529,0.0004050491,0.000013273457,0.0001556678,0.0000011364735],"about_ca_topic_score_codex":0.0057285,"about_ca_topic_score_gemma":0.009244557,"teacher_disagreement_score":0.0057285,"about_ca_system_score_codex":0.00021927935,"about_ca_system_score_gemma":0.00007570892,"threshold_uncertainty_score":0.011390328},"labels":[],"label_agreement":null},{"id":"W2981186968","doi":"10.3847/1538-4357/ab4ce9","title":"Droplets. II. Internal Velocity Structures and Potential Rotational Motions in Pressure-dominated Coherent Structures","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geophysics and Sensor Technology","field":"Engineering","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"","keywords":"Velocity gradient; Angular velocity; Rotation (mathematics); Rotation around a fixed axis; Group velocity; Relative velocity; Thermal velocity; Vector field; Gravitational potential","score_opus":0.003403411795490142,"score_gpt":0.19046361388433225,"score_spread":0.1870602020888421,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2981186968","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913924,0.00012157685,0.0065807775,0.00003844457,0.000008255549,0.000018126637,0.00021162632,0.00014814446,0.0014806557],"genre_scores_gemma":[0.9979232,0.000021932792,0.0017195714,0.0000061115675,0.0000051268803,0.0000047860485,0.00016586154,0.000023840264,0.00012967396],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999527,0.00000205804,0.000001921613,0.000014103143,0.000013009807,0.000016241907],"domain_scores_gemma":[0.9997868,0.00003641391,0.00006163126,0.000017469885,0.00005363683,0.000044141078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008803925,0.0001623053,0.00017522319,0.0010662092,0.0003161441,0.00047751484,0.0003052066,0.00016149913,0.0016152952],"category_scores_gemma":[0.000523452,0.00014348298,0.00019268774,0.00039739962,0.00029377025,0.0004898515,0.0003216183,0.00031411528,0.0002652604],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004483315,0.00020186235,0.2549888,0.00010121181,0.00009630474,0.0005376003,0.000547148,0.023916848,0.6645222,0.0045910785,0.0012726376,0.048776012],"study_design_scores_gemma":[0.0001054491,0.00026308943,0.70523494,0.00003093196,0.000053538068,0.00047566366,0.0004042331,0.20388333,0.08339504,0.0030212929,0.0030503476,0.00008217806],"about_ca_topic_score_codex":0.002466646,"about_ca_topic_score_gemma":0.0014717403,"teacher_disagreement_score":0.002466646,"about_ca_system_score_codex":0.0003927027,"about_ca_system_score_gemma":0.00014622312,"threshold_uncertainty_score":0.0054036975},"labels":[],"label_agreement":null},{"id":"W2981236769","doi":"10.3847/1538-4357/ab59d5","title":"Testing the Spectroscopic Extraction of Suppression of Convective Blueshift","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Heliophysics Division; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Université de Genève; Queen's University Belfast; University of St Andrews; Scottish Universities Physics Alliance; California Institute of Technology; European Commission; Queen's University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; NASA Exoplanet Science Institute; Harvard University; National Aeronautics and Space Administration; John Templeton Foundation; Smithsonian Institution; National Science Foundation","keywords":"Blueshift; Exoplanet; Convection; Planet; Solar telescope; Spectrograph","score_opus":0.022293595796894605,"score_gpt":0.25349198759364017,"score_spread":0.23119839179674556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2981236769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9824982,0.00015374813,0.014329768,0.000050503764,0.000017429098,0.000036814316,0.0010149691,0.00024165242,0.0016569167],"genre_scores_gemma":[0.9924568,0.000033071457,0.0063527944,0.000023808829,0.000010770575,0.00002043192,0.00078513334,0.00003927554,0.0002780829],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994523,0.00010563105,0.000045641274,0.00022881613,0.00011965755,0.000048008413],"domain_scores_gemma":[0.99831855,0.00054605294,0.00035455805,0.00027997675,0.00036220526,0.00013869903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011879185,0.0004358223,0.00022994894,0.0012703513,0.0002481622,0.0005876024,0.00037524465,0.00046333284,0.00077926175],"category_scores_gemma":[0.003745127,0.00018751348,0.0004505324,0.00066457497,0.00017216578,0.00044853316,0.00054425607,0.00025131973,0.0005734234],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039804805,0.00021337414,0.85969174,0.00009878997,0.000324113,0.000083286344,0.00026186788,0.0044818544,0.081311956,0.0001761582,0.00042791056,0.05253091],"study_design_scores_gemma":[0.000022521623,0.00012266246,0.93846023,0.000013026686,0.00009456275,0.000102383114,0.00010379052,0.03521254,0.024567075,0.00014151553,0.001141973,0.000017633412],"about_ca_topic_score_codex":0.0045906464,"about_ca_topic_score_gemma":0.00596491,"teacher_disagreement_score":0.0045906464,"about_ca_system_score_codex":0.00029795818,"about_ca_system_score_gemma":0.0002159144,"threshold_uncertainty_score":0.009127855},"labels":[],"label_agreement":null},{"id":"W2981465730","doi":"10.3847/1538-4357/ab50c2","title":"The Gas–Star Formation Cycle in Nearby Star-forming Galaxies. I. Assessment of Multi-scale Variations","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Institut National de Physique Nucléaire et de Physique des Particules; National Institutes of Natural Sciences; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Natural Sciences and Engineering Research Council of Canada; National Science Council; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; European Commission; National Science Foundation; European Space Agency; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory","keywords":"Star formation; Galaxy; Galaxy formation and evolution; Resolution (logic); Image resolution; Galaxy merger; Scale (ratio)","score_opus":0.01000928271324376,"score_gpt":0.2609478036806088,"score_spread":0.2509385209673651,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2981465730","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988582,0.00013175035,0.00048399257,0.000009875604,0.0000010513974,0.0000064536002,0.00019507439,0.000014125159,0.00029950612],"genre_scores_gemma":[0.9992724,0.000019149558,0.000493058,0.000002890373,0.0000022479248,0.0000041300777,0.00013188191,0.0000024827907,0.00007167151],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998876,0.000026432395,0.000008539233,0.000032826825,0.00002798978,0.00001660327],"domain_scores_gemma":[0.9991603,0.00021384662,0.00031645046,0.0000985854,0.0000733581,0.00013747011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003871691,0.00012243536,0.00017070277,0.0016804537,0.0002104763,0.0004209711,0.0001955971,0.0002246782,0.0005963857],"category_scores_gemma":[0.0011549356,0.00010148089,0.00018568747,0.001040893,0.00027091766,0.0004059511,0.00040055017,0.00015857405,0.00010534073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011542342,0.000028585951,0.9732484,0.000019670459,0.00005234547,0.000068500995,0.00017975926,0.0013978566,0.014778425,0.00017713344,0.00006310932,0.009870844],"study_design_scores_gemma":[0.0000013562079,0.000019791936,0.99700004,7.69669e-7,0.0000035791038,0.000029508974,0.000047093185,0.002283774,0.00045605903,0.000056712717,0.00009879137,0.0000025683762],"about_ca_topic_score_codex":0.006186892,"about_ca_topic_score_gemma":0.0075298566,"teacher_disagreement_score":0.006186892,"about_ca_system_score_codex":0.00032357345,"about_ca_system_score_gemma":0.00010111855,"threshold_uncertainty_score":0.012301803},"labels":[],"label_agreement":null},{"id":"W2981733279","doi":"10.3847/1538-4357/ab4c2e","title":"Probing Structure in Cold Gas at z ≲ 1 with Gravitationally Lensed Quasar Sight Lines","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration","keywords":"Quasar; Galaxy; Redshift; Line-of-sight; Lens (geology); Line (geometry); Doubly ionized oxygen; Sky; Spectroscopy","score_opus":0.005028383460712664,"score_gpt":0.1944064741202684,"score_spread":0.18937809065955574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2981733279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99947995,0.000023401984,0.00008352336,0.000006377078,5.593259e-7,0.0000015677934,0.00012645818,0.00000918682,0.00026905342],"genre_scores_gemma":[0.99950314,0.000009639973,0.00014662543,0.00000866676,0.0000025819797,0.0000013770243,0.0002379101,0.0000016910735,0.000088388384],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990106,0.000008564239,0.000004461237,0.000032971027,0.00001886248,0.000034138866],"domain_scores_gemma":[0.99940634,0.00007515763,0.00026089756,0.000036138143,0.00005199597,0.0001695638],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022195201,0.00021021676,0.00016676245,0.001033207,0.0002565242,0.0003702604,0.00026983445,0.00019589573,0.001132226],"category_scores_gemma":[0.00038472953,0.00014740632,0.00016467071,0.00056975253,0.0002620776,0.00030833308,0.00045309693,0.00020550478,0.00016406919],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000091523885,0.000027341854,0.97193944,0.000007937303,0.00003501528,0.00009146674,0.00018026892,0.00014989596,0.025179846,0.000059732964,0.00009688714,0.002140629],"study_design_scores_gemma":[0.0000012295794,0.000013884193,0.9994134,6.194658e-7,0.0000036437727,0.00002499019,0.000037716,0.00009732109,0.00034121596,0.000010970352,0.000054092696,9.051628e-7],"about_ca_topic_score_codex":0.0072131064,"about_ca_topic_score_gemma":0.010833804,"teacher_disagreement_score":0.0072131064,"about_ca_system_score_codex":0.00034249257,"about_ca_system_score_gemma":0.00007217907,"threshold_uncertainty_score":0.014342248},"labels":[],"label_agreement":null},{"id":"W2982193267","doi":"10.3847/1538-4357/aba001","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: The Hβ Radius–Luminosity Relation","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":70,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; York University; Office of Science; Johns Hopkins University; Science and Technology Facilities Council; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Reverberation mapping; Astrophysics; Physics; Quasar; Sky; Luminosity; RADIUS; Active galactic nucleus; Black hole (networking); Astronomy; Effective radius; Galaxy","score_opus":0.01868679364451803,"score_gpt":0.21549351380050613,"score_spread":0.1968067201559881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982193267","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9878279,0.0005185753,0.0024626984,0.0003398491,0.000011301186,0.000011113029,0.0047774557,0.00017323281,0.0038778798],"genre_scores_gemma":[0.99382305,0.00010617213,0.00094930455,0.000041192983,0.000012217347,0.000005908689,0.0047815493,0.000046135938,0.00023441607],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992298,0.00025977608,0.00003805096,0.00021643916,0.0001870922,0.000068827314],"domain_scores_gemma":[0.9913794,0.002124601,0.003147685,0.0011950021,0.0015948785,0.0005585586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021218674,0.00024005234,0.00018108456,0.0010103019,0.00018257766,0.0009397639,0.00038055654,0.00025255294,0.0010077942],"category_scores_gemma":[0.008371111,0.00014470982,0.00016201676,0.0010272401,0.0003526433,0.0006194557,0.00069078995,0.00027085826,0.0005885252],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042334417,0.000009333845,0.9879105,0.00001601355,0.00008343367,0.000031358606,0.0001208239,0.0033072317,0.00032838862,0.00046535343,0.0020368686,0.0056483266],"study_design_scores_gemma":[0.0000045622714,0.000010422826,0.9911885,0.000007124947,0.000012537964,0.000047630358,0.000059468035,0.0066477563,0.00029774397,0.00034141433,0.0013760723,0.000006712868],"about_ca_topic_score_codex":0.016724452,"about_ca_topic_score_gemma":0.010557754,"teacher_disagreement_score":0.016724452,"about_ca_system_score_codex":0.00043828491,"about_ca_system_score_gemma":0.00021179265,"threshold_uncertainty_score":0.033254266},"labels":[],"label_agreement":null},{"id":"W2982288820","doi":"10.3847/1538-4357/ab88a8","title":"The Dragonfly Wide Field Survey. I. Telescope, Survey Design, and Data Characterization","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Sky; Surface brightness; Dragonfly; Milky Way; Telescope; Galaxy; Brightness","score_opus":0.03149131334449308,"score_gpt":0.24276808515523499,"score_spread":0.2112767718107419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982288820","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.42355058,0.0026794095,0.12722482,0.0015983136,0.00020943898,0.009585167,0.3434984,0.013582841,0.07807108],"genre_scores_gemma":[0.3738249,0.001008807,0.28689495,0.0012178657,0.00031458156,0.008754772,0.29418805,0.0013668032,0.032429338],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9993895,0.000097971926,0.00002679972,0.00019461666,0.0001784786,0.000112644826],"domain_scores_gemma":[0.9994204,0.000066560184,0.00007728092,0.00017987864,0.00013477365,0.00012116489],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078787684,0.00061510445,0.0002840894,0.0023311214,0.00067257043,0.0006139635,0.0008787827,0.00035798637,0.007115817],"category_scores_gemma":[0.00086607673,0.0005600642,0.0001996343,0.0017797338,0.00034850443,0.00055427675,0.00086675823,0.00032355738,0.0041552573],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076326355,0.00021945793,0.23125024,0.0005867163,0.00009696318,0.00035070986,0.0006790471,0.0063253785,0.0667177,0.0045197727,0.18510967,0.50338113],"study_design_scores_gemma":[0.00021730071,0.00040398698,0.56928563,0.00013359169,0.00005436389,0.00063192204,0.00031980607,0.009409623,0.017073197,0.0017854472,0.40057507,0.00010999762],"about_ca_topic_score_codex":0.031023806,"about_ca_topic_score_gemma":0.048772965,"teacher_disagreement_score":0.031023806,"about_ca_system_score_codex":0.0013878292,"about_ca_system_score_gemma":0.001056,"threshold_uncertainty_score":0.061686456},"labels":[],"label_agreement":null},{"id":"W2982309009","doi":"10.3847/1538-4357/ab464c","title":"Anatomy of a Cooling Flow: The Feedback Response to Pure Cooling in the Core of the Phoenix Cluster","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of Waterloo","funders":"Space Telescope Science Institute; High Energy Physics; Smithsonian Astrophysical Observatory; U.S. Department of Energy; Princeton University; Office of Science; National Aeronautics and Space Administration; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Smithsonian Institution; National Science Foundation","keywords":"Cooling flow; Intracluster medium; Protein filament; Cluster (spacecraft); Core (optical fiber); Phoenix; Inner core; Galaxy cluster","score_opus":0.007872133330087376,"score_gpt":0.2341641380582378,"score_spread":0.22629200472815042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982309009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997311,0.00004364826,0.0010591527,0.00007239582,0.000003702972,0.00000898556,0.00008267145,0.00011298975,0.0013055562],"genre_scores_gemma":[0.9991447,0.000017772709,0.0003349309,0.000017702238,0.000007282839,0.0000046344935,0.00004348013,0.000016361655,0.0004131477],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995923,0.000004745169,0.0000011087109,0.000011895703,0.0000072260227,0.000015771844],"domain_scores_gemma":[0.9998449,0.00003333596,0.000026906504,0.000018636381,0.000025290909,0.000050894036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000100081474,0.00020571612,0.00019048867,0.0003242939,0.00035953283,0.00037572862,0.00032927791,0.00021335838,0.0013686391],"category_scores_gemma":[0.0005104097,0.00019302277,0.00013264443,0.00012875505,0.0003664081,0.0003954117,0.0005077406,0.00025064038,0.00016134106],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010149224,0.00015853239,0.15559271,0.00010276574,0.00008677411,0.0011512813,0.0013724645,0.020040445,0.78839093,0.0041627176,0.0019163343,0.026010152],"study_design_scores_gemma":[0.00007255426,0.0002916493,0.89144963,0.0000223115,0.00003321973,0.00025988955,0.000352192,0.06816594,0.034062892,0.0022136732,0.0030265104,0.000049484035],"about_ca_topic_score_codex":0.00646628,"about_ca_topic_score_gemma":0.0035030558,"teacher_disagreement_score":0.00646628,"about_ca_system_score_codex":0.0005581508,"about_ca_system_score_gemma":0.00019193519,"threshold_uncertainty_score":0.012857258},"labels":[],"label_agreement":null},{"id":"W2982473518","doi":"10.3847/1538-4357/ab53d3","title":"Metallicity Structure in the Milky Way Disk Revealed by Galactic H ii Regions","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"","keywords":"Milky Way; Metallicity; Galactic Center; Interstellar medium; Line (geometry); Maser; Disc","score_opus":0.008302024240907244,"score_gpt":0.21818089042929747,"score_spread":0.20987886618839025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2982473518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997458,0.00005676855,0.000026380952,0.0000032891342,3.223633e-7,4.511465e-7,0.000044377488,0.000002349634,0.000120286575],"genre_scores_gemma":[0.9997675,0.000023292785,0.000044388184,0.000002844429,0.0000011147742,7.799527e-7,0.00010630092,0.0000015961995,0.000052300275],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999069,0.000009358735,0.000007903681,0.000036338002,0.000017651068,0.000021883701],"domain_scores_gemma":[0.99957293,0.00006127679,0.00018549926,0.000040153045,0.00005666468,0.00008338182],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001299157,0.00015603175,0.00024279286,0.0011508508,0.00019245234,0.00058380875,0.00019276327,0.00019286659,0.0007274436],"category_scores_gemma":[0.0005325736,0.00013870966,0.00015199259,0.00070850604,0.00024728285,0.0002924549,0.0005748402,0.00009566737,0.00017243176],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079422854,0.000009538695,0.98133665,0.000009291527,0.00003960151,0.000088683075,0.00020132452,0.00012997496,0.015564709,0.00004495414,0.000039095703,0.0024568029],"study_design_scores_gemma":[0.0000012019357,0.0000085012325,0.99921966,0.0000012760955,0.0000062882827,0.00004347282,0.000093773764,0.000100917154,0.0004476897,0.00001620031,0.000059924558,0.0000012003595],"about_ca_topic_score_codex":0.002524542,"about_ca_topic_score_gemma":0.0027687857,"teacher_disagreement_score":0.002524542,"about_ca_system_score_codex":0.00020811355,"about_ca_system_score_gemma":0.0000746569,"threshold_uncertainty_score":0.0050197244},"labels":[],"label_agreement":null},{"id":"W2983226862","doi":"10.3847/1538-4357/ab3eb9","title":"Spatially Resolved Stellar Kinematics of the Ultra-diffuse Galaxy Dragonfly 44. II. Constraints on Fuzzy Dark Matter","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Australian Research Council; NASA Exoplanet Science Institute; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Dark matter; Galaxy; Halo; Dark matter halo; Galaxy rotation curve; Spiral galaxy; Galaxy formation and evolution; Astronomy","score_opus":0.006943177882909909,"score_gpt":0.2097252262566886,"score_spread":0.2027820483737787,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2983226862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987777,0.000025100486,0.0003834243,0.000028402896,7.1831676e-7,0.0000014082816,0.000034049914,0.000011829975,0.0007373691],"genre_scores_gemma":[0.9997696,0.000007970283,0.000121728386,0.0000037806435,8.124588e-7,3.8947226e-7,0.000032435975,0.0000012755456,0.000061891595],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996495,0.000004780899,8.671462e-7,0.000011840922,0.000006226542,0.000011401223],"domain_scores_gemma":[0.99982065,0.000028807131,0.000045766687,0.000024614423,0.000013261374,0.00006690084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010877984,0.0002049004,0.00022985796,0.00042364805,0.00028483523,0.00036514053,0.000357536,0.00024931596,0.0010623174],"category_scores_gemma":[0.0003222045,0.00017873,0.00014981555,0.00018833806,0.00036268562,0.00024708323,0.00055492006,0.00022880797,0.000119701035],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036434233,0.00008002463,0.83764875,0.000057136942,0.00012496006,0.0007597607,0.0007936111,0.057978887,0.081006214,0.0099541,0.00074086495,0.010491444],"study_design_scores_gemma":[0.000019524357,0.00009192136,0.89256537,0.000011656381,0.000034497116,0.00016910424,0.00031358172,0.10055962,0.0028210557,0.0025206758,0.00086765364,0.000025319654],"about_ca_topic_score_codex":0.011077779,"about_ca_topic_score_gemma":0.017484777,"teacher_disagreement_score":0.011077779,"about_ca_system_score_codex":0.0007932247,"about_ca_system_score_gemma":0.00015967012,"threshold_uncertainty_score":0.022026598},"labels":[],"label_agreement":null},{"id":"W2983397549","doi":"10.3847/1538-4357/ab5363","title":"Prompt X-Ray Emission from Fast Radio Bursts—Upper Limits with AstroSat","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Flux (metallurgy); Range (aeronautics); Energy (signal processing); Fluence; Yield (engineering); Cadmium zinc telluride; High energy","score_opus":0.013739692529788218,"score_gpt":0.27708462129046285,"score_spread":0.2633449287606746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2983397549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93464595,0.0032184203,0.039034545,0.00022289912,0.000027985809,0.000057485067,0.0020954837,0.0005460662,0.020151211],"genre_scores_gemma":[0.98814195,0.00037945312,0.008815296,0.000049358743,0.00003230318,0.000030146308,0.0017273811,0.000034119184,0.0007899839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99883467,0.00031895805,0.00008009818,0.00021775973,0.00040471047,0.00014374878],"domain_scores_gemma":[0.9872169,0.009315625,0.0011391178,0.0014049421,0.0006315641,0.00029180694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028849563,0.0007066338,0.00041716223,0.0026637525,0.0002889762,0.001449531,0.0007544344,0.0005818118,0.0025496534],"category_scores_gemma":[0.007661454,0.00034689493,0.0005292216,0.0012022032,0.00047475108,0.0012107095,0.0009258915,0.00046777993,0.00059654395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000909497,0.00015128574,0.9124339,0.0002154646,0.00019621942,0.00024459176,0.00029929934,0.026448585,0.016133314,0.006606995,0.0010686273,0.03529214],"study_design_scores_gemma":[0.000059691793,0.00031855225,0.8420624,0.00018294087,0.00017709893,0.00069427915,0.00034961308,0.113636084,0.026164604,0.008753529,0.0075255134,0.00007572928],"about_ca_topic_score_codex":0.00336127,"about_ca_topic_score_gemma":0.0030195364,"teacher_disagreement_score":0.00336127,"about_ca_system_score_codex":0.00058501447,"about_ca_system_score_gemma":0.0001762208,"threshold_uncertainty_score":0.015257299},"labels":[],"label_agreement":null},{"id":"W2983581670","doi":"10.3847/1538-4357/ab5521","title":"The Canada–France Imaging Survey: Reconstructing the Milky Way Star Formation History from Its White Dwarf Population","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; Université de Montréal; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Physics; Milky Way; White dwarf; Astrophysics; Population; Astronomy; Star formation; Dwarf spheroidal galaxy; Photometry (optics); Stars; Local Group; Dwarf galaxy; Galaxy; Demography","score_opus":0.010110829333240546,"score_gpt":0.19259666380839432,"score_spread":0.1824858344751538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2983581670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922652,0.00011214375,0.002695348,0.00006146765,0.0000026281236,0.000016988739,0.003023448,0.00019472365,0.0016279952],"genre_scores_gemma":[0.9905158,0.000048175454,0.004536341,0.000018859448,0.0000033757256,0.000009511711,0.004123049,0.00002629438,0.000718555],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986446,0.000023119823,0.000004281945,0.000041879564,0.000033658172,0.000032632674],"domain_scores_gemma":[0.99956435,0.000066402186,0.00007562532,0.000043202752,0.00017417535,0.00007614327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003321907,0.00024274911,0.00012647518,0.0011575281,0.00032417366,0.0004725976,0.00028577584,0.0001559269,0.0008096961],"category_scores_gemma":[0.00085561076,0.00012969883,0.00025892782,0.0008302321,0.000121570745,0.00015563442,0.00025633836,0.000103795406,0.00026241213],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006102661,0.000012718084,0.97078943,0.000012034054,0.00006752028,0.00006618995,0.00012326831,0.0078557255,0.003761494,0.00035549703,0.0014907107,0.015404419],"study_design_scores_gemma":[0.000010125017,0.0000134856555,0.95681965,0.000007732433,0.000023657118,0.000036095236,0.00014966668,0.037206404,0.0015236533,0.0000891932,0.0041096215,0.000010714188],"about_ca_topic_score_codex":0.8182771,"about_ca_topic_score_gemma":0.8851244,"teacher_disagreement_score":0.8182771,"about_ca_system_score_codex":0.002612203,"about_ca_system_score_gemma":0.0023994355,"threshold_uncertainty_score":0.3655861},"labels":[],"label_agreement":null},{"id":"W2983637971","doi":"10.3847/1538-4357/ab55db","title":"Consequences of Energetic Magnetar-like Outbursts of Nearby Neutron Stars: <sup>14</sup>C Events and the Cosmic Electron Spectrum","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute","funders":"National Natural Science Foundation of China","keywords":"Physics; Magnetar; Neutron star; Astrophysics; Pulsar; Astronomy; Cosmic ray; Electron; Magnetosphere; Vela; Heliosphere; Cosmic ray spallation; Nuclear physics; Ultra-high-energy cosmic ray; Solar wind; Plasma","score_opus":0.0045386960112418885,"score_gpt":0.20062048514204273,"score_spread":0.19608178913080085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2983637971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99932957,0.00007855294,0.00004416779,0.00004101877,0.0000063050925,0.0000016007615,0.00004387371,0.0000047324897,0.00045016894],"genre_scores_gemma":[0.9997279,0.000038835307,0.00003629849,0.000025279676,0.00000388187,9.870039e-7,0.000068728434,0.0000022207464,0.00009585978],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998734,0.000028144601,0.000010650656,0.000029779969,0.000027550112,0.000030494088],"domain_scores_gemma":[0.99921227,0.000117207615,0.00033639732,0.00006198654,0.00007455287,0.00019754253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025157793,0.00020426253,0.00022149348,0.00021493057,0.00055440224,0.000580905,0.00017926334,0.0004683504,0.0010444372],"category_scores_gemma":[0.0006920046,0.00010448807,0.00016496523,0.00018656683,0.00036725172,0.00017865894,0.00058275,0.00042194902,0.00014869875],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019638112,0.00015803386,0.88251084,0.000040616844,0.000113280854,0.0036800888,0.00017370649,0.00071761466,0.10440957,0.00044306475,0.0004555531,0.0053338213],"study_design_scores_gemma":[0.00002474073,0.00026307916,0.98649627,0.000007180392,0.000031078147,0.0019878987,0.00025970244,0.0006271498,0.009195668,0.00034914853,0.0007506072,0.0000074934337],"about_ca_topic_score_codex":0.0017706024,"about_ca_topic_score_gemma":0.0016318619,"teacher_disagreement_score":0.0017706024,"about_ca_system_score_codex":0.0002959354,"about_ca_system_score_gemma":0.00010759573,"threshold_uncertainty_score":0.003520608},"labels":[],"label_agreement":null},{"id":"W2984447553","doi":"10.3847/1538-4357/ab4ae2","title":"Search for Sources of Astrophysical Neutrinos Using Seven Years of IceCube Cascade Events","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Science and Technology Facilities Council","keywords":"Neutrino; Sky; Cascade; Muon; Context (archaeology); Neutrino detector; Muon neutrino; Neutrino astronomy","score_opus":0.015593491969416676,"score_gpt":0.2587770404610144,"score_spread":0.24318354849159773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2984447553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9881594,0.00011475394,0.0026646252,0.000054238237,0.000015855527,0.00008525056,0.0029417726,0.00012650422,0.005837537],"genre_scores_gemma":[0.9904467,0.00006293044,0.0025651131,0.000026317053,0.00002151129,0.000042168747,0.0064157867,0.000024966626,0.00039461558],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993333,0.00013272448,0.000029803676,0.00020708678,0.00013893115,0.00015813006],"domain_scores_gemma":[0.99870455,0.00033033252,0.00032205565,0.00018497011,0.0002403901,0.00021776461],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012192143,0.0005902903,0.0005075439,0.0015041763,0.0007224779,0.0009550123,0.00049162697,0.0004197227,0.0023864883],"category_scores_gemma":[0.0010829525,0.0003011011,0.0006799411,0.0010897648,0.00032872433,0.000528457,0.0010283015,0.00051339564,0.00033332995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0046462486,0.0008936796,0.83250123,0.00015996762,0.0008134571,0.0011967596,0.00047432104,0.012862441,0.10530619,0.0044349297,0.0030278135,0.033683073],"study_design_scores_gemma":[0.00030131446,0.0012904376,0.8868216,0.000052707397,0.0004315554,0.00086643896,0.00033586484,0.037939735,0.056261044,0.0015958912,0.01400346,0.00009990094],"about_ca_topic_score_codex":0.00531874,"about_ca_topic_score_gemma":0.012150547,"teacher_disagreement_score":0.00531874,"about_ca_system_score_codex":0.0006508199,"about_ca_system_score_gemma":0.00044246178,"threshold_uncertainty_score":0.010575533},"labels":[],"label_agreement":null},{"id":"W298464080","doi":"10.1088/0004-637x/811/2/101","title":"THE 3D FLOW FIELD AROUND AN EMBEDDED PLANET","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; The Scarborough Hospital; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Planet; Hydrostatic equilibrium; Vortex; Accretion (finance); Flow (mathematics); Field (mathematics); Magnetic field","score_opus":0.017548080316708955,"score_gpt":0.25677982703703156,"score_spread":0.2392317467203226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W298464080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9783317,0.000066851746,0.011226655,0.00032450317,0.000034608915,0.000039816117,0.0006615509,0.0003159831,0.008998443],"genre_scores_gemma":[0.9934136,0.000052358697,0.004980876,0.00006772734,0.000011765522,0.000021844071,0.00035065447,0.00003505879,0.0010661024],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999497,0.000008511696,0.0000017947222,0.000011302845,0.0000129223945,0.000015861744],"domain_scores_gemma":[0.99988997,0.000030873805,0.000016749882,0.000008382767,0.000020487323,0.000033458273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008344191,0.0002501815,0.00024538703,0.00040809892,0.00062638073,0.00075213844,0.00040758186,0.0007506272,0.0023613507],"category_scores_gemma":[0.00049106847,0.00019438953,0.00036837044,0.00036172554,0.00071409234,0.00043642882,0.00049342646,0.00036903564,0.00015546176],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012310532,0.00009572707,0.012414903,0.000027640737,0.000027227912,0.00045110952,0.00020228945,0.96782637,0.0076868082,0.005211986,0.00092543085,0.0050075217],"study_design_scores_gemma":[0.00003140272,0.000031475876,0.0067167273,0.0000057661546,0.0000062462336,0.00005680325,0.00008353639,0.9906542,0.0006359891,0.0011294311,0.00063345884,0.000015051362],"about_ca_topic_score_codex":0.016785655,"about_ca_topic_score_gemma":0.006726471,"teacher_disagreement_score":0.016785655,"about_ca_system_score_codex":0.0008745456,"about_ca_system_score_gemma":0.0008544319,"threshold_uncertainty_score":0.03337592},"labels":[],"label_agreement":null},{"id":"W2984854956","doi":"10.3847/1538-4357/ab76d0","title":"Multi-epoch Modeling of TXS 0506+056 and Implications for Long-term High-energy Neutrino Emission","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto","funders":"","keywords":"Blazar; Neutrino; Muon; Neutrino detector; Flux (metallurgy); Compton scattering; Sterile neutrino; Neutrino astronomy; Photon","score_opus":0.023061372446554606,"score_gpt":0.25464961005274533,"score_spread":0.23158823760619074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2984854956","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9875731,0.00013384191,0.007332307,0.0003492932,0.000032923126,0.000021536402,0.0008558048,0.00014961849,0.0035514638],"genre_scores_gemma":[0.9956923,0.000080498685,0.0021461074,0.00006593436,0.000022871998,0.000020955844,0.0008895242,0.00006764409,0.0010141875],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998247,0.00003946262,0.000010729758,0.000049021102,0.00003374197,0.000042333417],"domain_scores_gemma":[0.9994816,0.00015998253,0.000120477256,0.000060024588,0.0000782195,0.00009980241],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078790163,0.00052682246,0.0004581102,0.0006921887,0.00066302874,0.0014147796,0.0013019243,0.00079746713,0.0018125612],"category_scores_gemma":[0.0015880096,0.0004045642,0.0014979965,0.00072882447,0.0005734261,0.00084850716,0.0006503332,0.00071101484,0.00024205275],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011865341,0.000079196696,0.09409254,0.00002453942,0.00012253574,0.00022479129,0.00008689798,0.8961968,0.0025606502,0.004041519,0.00046794437,0.001983951],"study_design_scores_gemma":[0.000025991709,0.000032353775,0.023977429,0.00000768622,0.00003010313,0.00006783638,0.000036778107,0.9737301,0.00046175765,0.0009895928,0.0006213051,0.000019159072],"about_ca_topic_score_codex":0.042744454,"about_ca_topic_score_gemma":0.01973692,"teacher_disagreement_score":0.042744454,"about_ca_system_score_codex":0.001839116,"about_ca_system_score_gemma":0.0008807203,"threshold_uncertainty_score":0.084991336},"labels":[],"label_agreement":null},{"id":"W2984870007","doi":"10.3847/1538-4357/ab557c","title":"Estimating the Molecular Gas Mass of Low-redshift Galaxies from a Combination of Mid-infrared Luminosity and Optical Properties","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Natural Science Foundation of China","keywords":"Galaxy; Luminosity; Estimator; Observatory; Stellar mass; Luminous infrared galaxy; Spectroscopy; Extragalactic astronomy","score_opus":0.005919513635153021,"score_gpt":0.19214747442921787,"score_spread":0.18622796079406484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2984870007","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984534,0.00009964518,0.0010390388,0.000010726339,7.7482827e-7,0.000003601158,0.00023185417,0.000030825864,0.00012995933],"genre_scores_gemma":[0.9986236,0.000027469296,0.0008328035,0.000005690258,0.0000047913672,0.0000034041755,0.00043108183,0.000004745877,0.00006645399],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99975234,0.00005033622,0.000014257823,0.00008428871,0.000058388814,0.00004037484],"domain_scores_gemma":[0.9984725,0.00037725188,0.000603831,0.00017792803,0.00017787138,0.00019059985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081214367,0.00036184557,0.00040987154,0.0022825208,0.00022813812,0.00095436565,0.00044507903,0.00034734164,0.0006057422],"category_scores_gemma":[0.0019167325,0.00025790313,0.00025581857,0.00088056846,0.00029087046,0.0004846012,0.00054302486,0.00017910702,0.00046064256],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003242167,0.000013533911,0.99242413,0.000008019089,0.000030479716,0.000013592364,0.00002801426,0.00064486254,0.0040855897,0.00002130741,0.000032711752,0.002665157],"study_design_scores_gemma":[0.0000022124798,0.000017628066,0.99374264,0.0000033359343,0.000016827556,0.000032299187,0.000041416733,0.005037973,0.0009769179,0.000026842321,0.000096433636,0.0000054357924],"about_ca_topic_score_codex":0.0044185966,"about_ca_topic_score_gemma":0.0068548876,"teacher_disagreement_score":0.0044185966,"about_ca_system_score_codex":0.00035450378,"about_ca_system_score_gemma":0.00013483582,"threshold_uncertainty_score":0.008785784},"labels":[],"label_agreement":null},{"id":"W2984988422","doi":"10.3847/1538-4357/ab4817","title":"Measurement of the Extragalactic Background Light Spectral Energy Distribution with VERITAS","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Office of Science; National Energy Research Scientific Computing Center; National Science Foundation; Science Foundation Ireland; U.S. Department of Energy; Irish Centre for High-End Computing; Smithsonian Institution","keywords":"Blazar; Extragalactic background light; Spectral energy distribution; Photon; Spectral line; Radiative transfer; Background radiation; Infrared; Radiation; Cosmic infrared background","score_opus":0.007359209504451764,"score_gpt":0.1881510223285329,"score_spread":0.18079181282408113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2984988422","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98728496,0.00011970038,0.0033670135,0.0000319849,0.0000094027455,0.000016526363,0.0036273655,0.0003709381,0.0051719937],"genre_scores_gemma":[0.9867883,0.000078108125,0.005948257,0.000038952498,0.000014144181,0.000027277536,0.005431122,0.00006373917,0.0016101286],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994191,0.000071696726,0.000024355506,0.00021986493,0.00017900173,0.00008605839],"domain_scores_gemma":[0.9986651,0.00021490199,0.00045043477,0.00033392326,0.00018132702,0.00015429937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043026684,0.00032596834,0.00020897294,0.0017856983,0.00023265177,0.0006933305,0.00047114588,0.00022679866,0.003945137],"category_scores_gemma":[0.00082426536,0.00023013822,0.0002830121,0.0009769719,0.00026565345,0.0004396656,0.0008291099,0.00042887227,0.0007864187],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008426637,0.00012960198,0.75762326,0.00007946662,0.00034045847,0.00021521751,0.00037900274,0.0027698,0.19388977,0.0022790802,0.0018026861,0.039648954],"study_design_scores_gemma":[0.000037818525,0.00014924786,0.94850636,0.000017541734,0.000064782515,0.00024836278,0.00010529669,0.005837548,0.04021311,0.00034706693,0.004449729,0.000023221543],"about_ca_topic_score_codex":0.004598279,"about_ca_topic_score_gemma":0.007207433,"teacher_disagreement_score":0.004598279,"about_ca_system_score_codex":0.0004571475,"about_ca_system_score_gemma":0.00015610288,"threshold_uncertainty_score":0.013197839},"labels":[],"label_agreement":null},{"id":"W2985239367","doi":"10.3847/1538-4357/ab3e3f","title":"A Supernova Remnant Counterpart for HESS J1832−085","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Supernova remnant; Interstellar medium; Molecular cloud; Supernova; Spectral index; Near-Earth supernova; Hadron","score_opus":0.008553911026179643,"score_gpt":0.22828194780182456,"score_spread":0.21972803677564492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2985239367","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973379,0.000097802134,0.00008042122,0.000051513434,0.0000116866595,0.000009498741,0.0003130477,0.000034678975,0.0020636613],"genre_scores_gemma":[0.99884665,0.000029106064,0.000098449615,0.000027275164,0.000012674129,0.0000028773952,0.00050005445,0.000005340138,0.00047753908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995315,0.0000026005587,0.0000043475547,0.000010895305,0.000009647514,0.00001943432],"domain_scores_gemma":[0.9997377,0.000014020956,0.00007327207,0.0000252929,0.000021712665,0.00012805911],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010986661,0.0002480872,0.00016677359,0.00080262305,0.0004858713,0.00042899535,0.0002485939,0.0003484491,0.004234759],"category_scores_gemma":[0.00023659556,0.00010640239,0.00024079804,0.00047382608,0.00020557182,0.00014082211,0.00039747372,0.00019675156,0.0008408124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000845321,0.0002120175,0.87035894,0.00006080356,0.00012060237,0.06629543,0.000459928,0.00045859936,0.044711746,0.0010970829,0.002205527,0.013174087],"study_design_scores_gemma":[0.00005883917,0.00031467906,0.96366173,0.00001659621,0.00004455609,0.025198778,0.00041790344,0.00068205217,0.0032451623,0.00032606468,0.006018358,0.00001533902],"about_ca_topic_score_codex":0.0049476433,"about_ca_topic_score_gemma":0.0059595373,"teacher_disagreement_score":0.0049476433,"about_ca_system_score_codex":0.00029132227,"about_ca_system_score_gemma":0.00014649218,"threshold_uncertainty_score":0.014166713},"labels":[],"label_agreement":null},{"id":"W2985245222","doi":"10.3847/1538-4357/ab536c","title":"The Distribution of Ultra-diffuse and Ultra-compact Galaxies in the Frontier Fields","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Galaxy; Galaxy cluster; Coma Cluster; Spatial distribution; RADIUS; Cluster (spacecraft); Mass distribution; Virial theorem; Stars","score_opus":0.005138372919486597,"score_gpt":0.2036966297108937,"score_spread":0.1985582567914071,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2985245222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996476,0.000051212217,0.000025915024,0.0000054520347,3.2958553e-7,6.300886e-7,0.000050773957,0.0000020044388,0.00021591458],"genre_scores_gemma":[0.99973637,0.000022644459,0.000026962685,0.0000035218877,0.0000019554514,6.7097534e-7,0.000103098726,6.4570906e-7,0.00010417803],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998503,0.000014644162,0.000007375473,0.000047373564,0.000026753738,0.00005362193],"domain_scores_gemma":[0.99899024,0.00014168644,0.0003408447,0.000090281006,0.00010994845,0.00032708142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022913216,0.00013436607,0.00016978868,0.0020450095,0.00026620566,0.00061264366,0.00030564892,0.000190543,0.0022284077],"category_scores_gemma":[0.00056761556,0.00009254707,0.00011640139,0.00066871,0.0005922579,0.00036357378,0.00066621613,0.00013507235,0.0002605362],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007584116,0.000015798707,0.9914259,0.000006487778,0.000019447389,0.000059609654,0.00028036343,0.00006945938,0.0046758223,0.00022383007,0.00010112729,0.0030463522],"study_design_scores_gemma":[0.0000019040989,0.000015406316,0.9993799,0.000001432773,0.00000296264,0.000063179155,0.00018981559,0.00007330706,0.0001230426,0.000031695574,0.000115753304,0.0000015238211],"about_ca_topic_score_codex":0.0053012385,"about_ca_topic_score_gemma":0.0068518138,"teacher_disagreement_score":0.0053012385,"about_ca_system_score_codex":0.00031911078,"about_ca_system_score_gemma":0.000086176085,"threshold_uncertainty_score":0.010540783},"labels":[],"label_agreement":null},{"id":"W2985406793","doi":"10.3847/1538-4357/ab46ab","title":"The M101 Satellite Luminosity Function and the Halo–Halo Scatter among Local Volume Hosts","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":95,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Local Group; Milky Way; Halo; Surface brightness; Astronomy; Luminosity; Population; Luminosity function; Stellar population; Star formation; Medicine","score_opus":0.003291216369137311,"score_gpt":0.17444852571364342,"score_spread":0.1711573093445061,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2985406793","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994066,0.000028611661,0.000073739546,0.000006854322,5.0185923e-7,6.4109724e-7,0.00008363822,0.0000070637993,0.00039248215],"genre_scores_gemma":[0.9996953,0.000008318625,0.00002879399,0.0000021551566,0.0000011305849,4.4056628e-7,0.0001494731,0.0000016752442,0.00011273476],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998963,0.000017281887,0.0000070493547,0.000023737746,0.000027151014,0.000028430746],"domain_scores_gemma":[0.99909663,0.00020639859,0.00027494642,0.0000867531,0.00009618484,0.00023900383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021691705,0.00015155003,0.00012944567,0.0010552241,0.0001999309,0.0008173426,0.00020697707,0.00015760763,0.0022044017],"category_scores_gemma":[0.0011566184,0.000077938195,0.000114725335,0.00053248176,0.0002557176,0.0003124299,0.00050681824,0.00011190987,0.0006155208],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054151504,0.000010626578,0.9937511,0.0000045134016,0.00002022915,0.0000556787,0.00011915257,0.0003610894,0.0023488952,0.00008969747,0.00009976964,0.003085092],"study_design_scores_gemma":[0.0000014850672,0.000025827354,0.9980318,0.0000021891053,0.000005597689,0.00014739994,0.00018833889,0.00085912185,0.0005240767,0.00004991469,0.00016226772,0.0000020326959],"about_ca_topic_score_codex":0.003824102,"about_ca_topic_score_gemma":0.0030894203,"teacher_disagreement_score":0.003824102,"about_ca_system_score_codex":0.00028088447,"about_ca_system_score_gemma":0.00007353108,"threshold_uncertainty_score":0.007603705},"labels":[],"label_agreement":null},{"id":"W2985688170","doi":"10.3847/1538-4357/ab49fb","title":"The Next Generation Virgo Cluster Survey. XVII. A Search for Planetary Nebulae in Virgo Cluster Globular Clusters","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Virgo Cluster; Globular cluster; Planetary nebula; Galaxy; Cluster (spacecraft); Star cluster; Local Group; Galaxy cluster","score_opus":0.030077929436288457,"score_gpt":0.2508569335230294,"score_spread":0.22077900408674095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2985688170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95611185,0.0017330679,0.0004510388,0.00039559908,0.000032036845,0.00010184494,0.036495022,0.0001041813,0.0045753564],"genre_scores_gemma":[0.94409287,0.0007079051,0.001534265,0.00026594094,0.000029365685,0.00009661826,0.049489733,0.000021958213,0.0037612463],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999845,0.000021771191,0.000010352579,0.000040398154,0.000040906252,0.000041468644],"domain_scores_gemma":[0.9995664,0.000030621846,0.000096237316,0.000044135304,0.00008021482,0.00018237815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037271372,0.00014200604,0.00013669558,0.0024081797,0.0002904407,0.00032731864,0.00031117248,0.00020399025,0.0017297635],"category_scores_gemma":[0.00053162774,0.000086611566,0.00016829805,0.0017447677,0.00009660039,0.00015646157,0.0005923067,0.00015992427,0.00049145217],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037412505,0.000011299404,0.98741025,0.000037159047,0.000043463595,0.000055852175,0.00009870862,0.00006323011,0.0015479246,0.000116331794,0.0028740207,0.0077042533],"study_design_scores_gemma":[0.0000015154782,0.0000045864886,0.9973398,0.000005752614,0.000006869997,0.000031181014,0.000040389656,0.000048031736,0.0000848615,0.000013261489,0.0024228767,8.9937544e-7],"about_ca_topic_score_codex":0.03347323,"about_ca_topic_score_gemma":0.052939624,"teacher_disagreement_score":0.03347323,"about_ca_system_score_codex":0.00044989143,"about_ca_system_score_gemma":0.00033274604,"threshold_uncertainty_score":0.06655675},"labels":[],"label_agreement":null},{"id":"W2985983322","doi":"10.3847/1538-4357/ab585a","title":"Modeling of the Variable Circumstellar Absorption Features of WD 1145+017","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Precession; Opacity; Absorption (acoustics); White dwarf; Phase (matter); Variable (mathematics); Radial velocity","score_opus":0.01393197578691254,"score_gpt":0.22143653871849656,"score_spread":0.207504562931584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2985983322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9849473,0.00013909374,0.009960966,0.00012156547,0.0000146936145,0.000022713099,0.00023087564,0.000083282874,0.0044795265],"genre_scores_gemma":[0.99832827,0.000037217804,0.0008507419,0.00001177916,0.000005088194,0.000010682357,0.000079737096,0.000014896615,0.0006615852],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994385,0.000012155081,0.000002375005,0.000014696825,0.000009136943,0.000017674747],"domain_scores_gemma":[0.9998547,0.000036322766,0.00002855668,0.000018848516,0.000021409678,0.00004001327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015023127,0.0003825451,0.0003562907,0.0003359767,0.0004010415,0.0005856976,0.0010811744,0.00091419194,0.0011401598],"category_scores_gemma":[0.00051931676,0.00025295225,0.00047360233,0.00023695789,0.0005321824,0.00046522348,0.0004307605,0.00030347815,0.00020319395],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007483196,0.0000441482,0.009083026,0.000019136593,0.000023783688,0.0003209638,0.000055689674,0.9830494,0.0042523146,0.0015274282,0.00016799386,0.0013812422],"study_design_scores_gemma":[0.000020827636,0.000024804862,0.0023292247,0.0000022980807,0.0000070840365,0.00003172533,0.000016000553,0.9968221,0.0003093046,0.00025538407,0.00017557648,0.0000056688727],"about_ca_topic_score_codex":0.022780564,"about_ca_topic_score_gemma":0.00729908,"teacher_disagreement_score":0.022780564,"about_ca_system_score_codex":0.0009591367,"about_ca_system_score_gemma":0.0005326947,"threshold_uncertainty_score":0.045295954},"labels":[],"label_agreement":null},{"id":"W2987145466","doi":"10.3847/1538-4357/ab4a01","title":"The SPIRITS Sample of Luminous Infrared Transients: Uncovering Hidden Supernovae and Dusty Stellar Outbursts in Nearby Galaxies*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Jet Propulsion Laboratory; Office of Science; Brookhaven National Laboratory; Ministério da Ciência, Tecnologia e Inovação; Lawrence Berkeley National Laboratory; Ministerio de Ciencia, Tecnología e Innovación Productiva; Commonwealth Scientific and Industrial Research Organisation; York University; Australian Government; Carnegie Mellon University; College of Engineering, Michigan State University; Goddard Space Flight Center; University of Washington; Alfred P. Sloan Foundation; Princeton University; Johns Hopkins University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Geographic Society; California Institute of Technology; U.S. Department of Energy; Universidad Nacional Autónoma de México; European Southern Observatory; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; W. M. Keck Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Astronomy; Galaxy; Infrared; Luminous infrared galaxy","score_opus":0.008098041523406919,"score_gpt":0.2140825795622081,"score_spread":0.20598453803880118,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2987145466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986889,0.000057122576,0.00006917919,0.000006130453,0.0000014915694,0.0000075837056,0.00090785895,0.000008561586,0.00025306144],"genre_scores_gemma":[0.99499476,0.00006729145,0.00027767455,0.000017155106,0.000009266346,0.000009714929,0.0044311755,0.0000065372583,0.0001864224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996165,0.000037413254,0.000051436164,0.000119802135,0.00010170927,0.00007305347],"domain_scores_gemma":[0.9982279,0.00012093816,0.00082500244,0.00033219438,0.00013721456,0.0003567887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005735598,0.00018324424,0.00027870826,0.002732379,0.00030252774,0.00061804854,0.00035730822,0.00015543967,0.0008860983],"category_scores_gemma":[0.0015609041,0.00014752711,0.0003543394,0.0013752367,0.00038625984,0.00036071418,0.0014239027,0.00014104976,0.00022941525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006905751,0.000021772536,0.9940491,0.000015145579,0.00004085268,0.00007641069,0.00016656873,0.0000650171,0.0021498962,0.000066105116,0.0002099258,0.003070139],"study_design_scores_gemma":[0.000005000615,0.00003507288,0.9986374,0.000007725813,0.000022226344,0.00016369614,0.00019166,0.00012690696,0.00024311463,0.000023983228,0.000541023,0.0000021747558],"about_ca_topic_score_codex":0.00341612,"about_ca_topic_score_gemma":0.007838622,"teacher_disagreement_score":0.00341612,"about_ca_system_score_codex":0.00021470465,"about_ca_system_score_gemma":0.00023736402,"threshold_uncertainty_score":0.0067924857},"labels":[],"label_agreement":null},{"id":"W2987251341","doi":"10.3847/1538-4357/ab4883","title":"Sensitivity of Super-Kamiokande with Gadolinium to Low Energy Antineutrinos from Pre-supernova Emission","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg; University of Regina; University of British Columbia; TRIUMF; University of Toronto","funders":"Science and Technology Facilities Council; National Research Foundation of Korea; National Natural Science Foundation of China","keywords":"Supernova; Neutrino; Red supergiant; Gadolinium; Neutrino detector; Detector; Low energy; Sensitivity (control systems); Type II supernova","score_opus":0.007645900542129403,"score_gpt":0.24719374642681644,"score_spread":0.23954784588468703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2987251341","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974866,0.00034162818,0.0007188432,0.000029447423,0.000014168725,0.000009077424,0.00013351637,0.000049975377,0.0012167862],"genre_scores_gemma":[0.99846184,0.00008858323,0.0004768109,0.000041857806,0.000005092418,0.000005840581,0.0002250143,0.000009553258,0.00068546535],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997224,0.00005135789,0.0000135821265,0.000075494085,0.000070188275,0.000066919594],"domain_scores_gemma":[0.99937385,0.00017759035,0.00017183308,0.00006334317,0.0001241824,0.00008925478],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051691337,0.00028850738,0.00018830753,0.0005622558,0.0001172032,0.0005626973,0.00036099076,0.0004689577,0.0011651325],"category_scores_gemma":[0.00085828005,0.00022213449,0.00026352936,0.00024333563,0.00019733116,0.00030364082,0.00057210826,0.00027004062,0.00034410885],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004196855,0.00016070467,0.37993625,0.00018208212,0.00038236656,0.000496446,0.00012012074,0.0021818173,0.59410244,0.00043300976,0.0004517404,0.017356116],"study_design_scores_gemma":[0.00010081092,0.0023564082,0.47474056,0.00005373475,0.00031878988,0.001153936,0.00020603804,0.011136777,0.50376946,0.0006404073,0.0054816008,0.00004143206],"about_ca_topic_score_codex":0.001038354,"about_ca_topic_score_gemma":0.0012929572,"teacher_disagreement_score":0.0011651325,"about_ca_system_score_codex":0.00022140521,"about_ca_system_score_gemma":0.00008732303,"threshold_uncertainty_score":0.0038977265},"labels":[],"label_agreement":null},{"id":"W2987578472","doi":"10.3847/1538-4357/ab4b47","title":"NuSTAR and Chandra Observations of New X-Ray Transients in the Central Parsec of the Galaxy","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Spectral line; Galaxy; Thermal; Reflection (computer programming); Ionization; Accretion (finance); Swift; Black hole (networking)","score_opus":0.017738018312526152,"score_gpt":0.2164848290376092,"score_spread":0.19874681072508305,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2987578472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998741,0.00009358646,0.00010478538,0.000010331576,0.0000028397367,0.0000037811142,0.00050070253,0.000053058506,0.0004899245],"genre_scores_gemma":[0.9961242,0.00006786047,0.0007261641,0.000026310316,0.000008846788,0.000008670893,0.0027646373,0.000022408463,0.00025084981],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998543,0.0000106432035,0.000009830802,0.000048333004,0.00004474794,0.00003216919],"domain_scores_gemma":[0.9993192,0.00006411843,0.00021862779,0.00009590599,0.000074206444,0.00022800002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002893244,0.0002063723,0.00038521638,0.0010292595,0.00035116682,0.0006529241,0.000290744,0.00022137712,0.0006597369],"category_scores_gemma":[0.00054036325,0.0002021967,0.00033417184,0.0007511646,0.00026052503,0.00031063714,0.0007812537,0.0003204452,0.00022779404],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010356018,0.00024642263,0.8751615,0.00012836012,0.0002443497,0.0012231808,0.0010384981,0.0017544223,0.09256226,0.00064565043,0.0019942196,0.023965567],"study_design_scores_gemma":[0.000010196449,0.000042056163,0.9973049,0.000004675751,0.000012946447,0.00019927109,0.000045006265,0.00064587453,0.00084456475,0.00003814219,0.0008450711,0.000007225595],"about_ca_topic_score_codex":0.003316613,"about_ca_topic_score_gemma":0.0064462847,"teacher_disagreement_score":0.003316613,"about_ca_system_score_codex":0.0003414104,"about_ca_system_score_gemma":0.00023917321,"threshold_uncertainty_score":0.0065945983},"labels":[],"label_agreement":null},{"id":"W2989408301","doi":"10.3847/1538-4357/ab9d85","title":"COSMIC Variance in Binary Population Synthesis","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":290,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Gravitational wave; Binary number; Population; Cosmic variance; Binary star; COSMIC cancer database; Observable","score_opus":0.014628120476690137,"score_gpt":0.22198062072404773,"score_spread":0.2073525002473576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2989408301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9130225,0.0003210071,0.06826656,0.00038972637,0.00010137821,0.00009048939,0.0017920524,0.0009516084,0.015064647],"genre_scores_gemma":[0.9882095,0.000061123006,0.009850093,0.00007921546,0.000016575208,0.000064576925,0.00069598237,0.00010394161,0.0009189684],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99962676,0.0001555394,0.000012853557,0.00007602394,0.00007164545,0.00005718298],"domain_scores_gemma":[0.9980635,0.0012324619,0.00014471039,0.00020878538,0.00023087593,0.000119713804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013532212,0.00034175153,0.0004808889,0.000704651,0.00050348334,0.0008822394,0.00084305555,0.0005408154,0.0024812592],"category_scores_gemma":[0.006693162,0.00023605724,0.0004997496,0.00057404186,0.00064642966,0.00068728044,0.0006346805,0.00062591967,0.00018781335],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000062657986,0.000031396696,0.015651805,0.00002885258,0.000054418426,0.00004335881,0.000055948938,0.961785,0.0007020863,0.01575046,0.0010488811,0.0047851694],"study_design_scores_gemma":[0.000023052604,0.000016044365,0.0015353293,0.000005386961,0.000011194333,0.0000144083115,0.000011036685,0.9933255,0.00055476197,0.0037594934,0.00073660846,0.000007140853],"about_ca_topic_score_codex":0.012603182,"about_ca_topic_score_gemma":0.008897585,"teacher_disagreement_score":0.012603182,"about_ca_system_score_codex":0.0011398401,"about_ca_system_score_gemma":0.00082389155,"threshold_uncertainty_score":0.02505964},"labels":[],"label_agreement":null},{"id":"W2990182115","doi":"10.3847/1538-4357/ab59de","title":"Probing the Properties of the Pulsar Wind in the Gamma-Ray Binary HESS J0632+057 with NuSTAR and VERITAS Observations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Office of Science; California Institute of Technology; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Pulsar; Astronomy; Binary number; Binary pulsar; Gamma ray; X-ray binary; Gamma-ray astronomy; Neutron star; Millisecond pulsar","score_opus":0.024252241475304234,"score_gpt":0.19726916597678298,"score_spread":0.17301692450147876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990182115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989868,0.00008046013,0.0001064941,0.000009013888,0.0000035967305,0.0000024325093,0.00029665264,0.000014145325,0.0005004529],"genre_scores_gemma":[0.99829274,0.000041760213,0.00039818473,0.0000067599376,0.00000707049,0.0000029655423,0.0010832618,0.000007388288,0.00015982852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985564,0.000016831418,0.0000101818,0.00004724086,0.00004328695,0.000026842717],"domain_scores_gemma":[0.99962986,0.00003922214,0.00013410959,0.00004608224,0.00005798194,0.00009267166],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002807969,0.00026495758,0.0002934856,0.0013684683,0.0002699716,0.00056527567,0.00019657718,0.00028091393,0.0007663892],"category_scores_gemma":[0.0004067776,0.0001903565,0.0002378055,0.0009067903,0.00018305109,0.00022398797,0.0005194284,0.00020344675,0.00026606687],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068042584,0.00011757338,0.82233816,0.000087153996,0.00017703311,0.0008905974,0.00033334194,0.0019582093,0.15937786,0.00036788508,0.00064605847,0.013025798],"study_design_scores_gemma":[0.00001546314,0.00009996905,0.9925527,0.000007334054,0.00003006612,0.00029202164,0.000094983276,0.0026905653,0.0034452374,0.000063292726,0.0007000112,0.000008397138],"about_ca_topic_score_codex":0.002064968,"about_ca_topic_score_gemma":0.0062957434,"teacher_disagreement_score":0.002064968,"about_ca_system_score_codex":0.00022813508,"about_ca_system_score_gemma":0.00014568452,"threshold_uncertainty_score":0.004105866},"labels":[],"label_agreement":null},{"id":"W2990188202","doi":"10.3847/1538-4357/ab4d58","title":"The Diffuse Ionized Gas Halo of the Small Magellanic Cloud","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of British Columbia","funders":"","keywords":"Halo; Galactic halo; Ionization; Small Magellanic Cloud; Plasma; Large Magellanic Cloud; Emission spectrum; Galaxy","score_opus":0.005749826556132739,"score_gpt":0.18701044434658376,"score_spread":0.18126061779045102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990188202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984366,0.00014040989,0.00021116449,0.000008761678,7.4389146e-7,0.0000022580614,0.00010538301,0.000010318562,0.0010843067],"genre_scores_gemma":[0.999532,0.00006174125,0.00012585297,0.0000032710154,0.00000170721,7.610195e-7,0.00011081274,0.0000014936518,0.00016235642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999629,0.000002955178,0.0000015501777,0.000009502131,0.000011546654,0.00001154247],"domain_scores_gemma":[0.9998834,0.0000121011435,0.0000484857,0.000009032998,0.00001404199,0.000032814984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007068907,0.00010926316,0.000067638735,0.00072017196,0.00023495252,0.00036916265,0.00016385922,0.0000577773,0.0010120248],"category_scores_gemma":[0.00018814352,0.00008194597,0.00006476905,0.000460397,0.00022878704,0.00018784952,0.00035345377,0.00006511405,0.000103388025],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010732932,0.000017630837,0.90295506,0.000035837376,0.00006915876,0.00032106639,0.0003222967,0.00037288954,0.08300594,0.0005890061,0.00023656887,0.011967178],"study_design_scores_gemma":[0.0000034923773,0.000016266724,0.9940196,0.0000079433285,0.000014899183,0.00020023296,0.00011694096,0.0003937571,0.0038663826,0.00009931533,0.001258737,0.0000023881264],"about_ca_topic_score_codex":0.011073105,"about_ca_topic_score_gemma":0.018929793,"teacher_disagreement_score":0.011073105,"about_ca_system_score_codex":0.00030649282,"about_ca_system_score_gemma":0.000115247465,"threshold_uncertainty_score":0.0220173},"labels":[],"label_agreement":null},{"id":"W2990247591","doi":"10.3847/1538-4357/ab571d","title":"Globular Cluster Systems and X-Ray Atmospheres in Galaxies*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Waterloo","funders":"","keywords":"Globular cluster; Dark matter; Galaxy; Galaxy cluster; Halo; Galaxy groups and clusters; Cluster (spacecraft); Stellar mass; RADIUS; Scaling","score_opus":0.004697293055435343,"score_gpt":0.19558170882586282,"score_spread":0.19088441577042747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990247591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992505,0.000079353704,0.000078453595,0.000030385272,0.0000010384574,9.4802823e-7,0.00008120005,0.00000614741,0.0004719719],"genre_scores_gemma":[0.9998149,0.000017846305,0.000035318804,0.0000033908268,0.0000017526555,4.282686e-7,0.00007692195,0.0000012873048,0.000048055703],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975675,0.00006600417,0.000018930286,0.000060568018,0.000059001784,0.000038683836],"domain_scores_gemma":[0.99608755,0.0014740274,0.0012625266,0.0003647731,0.00026971338,0.00054148404],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006921824,0.0001374938,0.00015017053,0.0012251688,0.0002987495,0.0009727079,0.00024340313,0.0002885949,0.0021334349],"category_scores_gemma":[0.00436713,0.00011559813,0.00019258102,0.0012228872,0.0006969294,0.00041190797,0.0008604189,0.0002309511,0.00027433145],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000015688875,0.0000068396157,0.9981358,0.0000032767641,0.000019448997,0.00001256722,0.00010739235,0.00045973255,0.00029979885,0.00020807059,0.000035156943,0.000696242],"study_design_scores_gemma":[7.704278e-7,0.0000050326485,0.99898666,0.0000015548294,0.0000038997296,0.000018092094,0.00004664448,0.00069460284,0.000052044717,0.00011024824,0.00007948649,0.0000010387646],"about_ca_topic_score_codex":0.010007389,"about_ca_topic_score_gemma":0.009044321,"teacher_disagreement_score":0.010007389,"about_ca_system_score_codex":0.0004939865,"about_ca_system_score_gemma":0.00014739114,"threshold_uncertainty_score":0.019898236},"labels":[],"label_agreement":null},{"id":"W2990377646","doi":"10.3847/1538-4357/ab9749","title":"Spitzer + VLTI-GRAVITY Measure the Lens Mass of a Nearby Microlensing Event","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Key Research and Development Program of China; Natural Science Foundation of Shandong Province; National Natural Science Foundation of China","keywords":"Gravitational microlensing; Einstein radius; Parallax; Lens (geology); Measure (data warehouse); Interferometry; Microlens; Light curve; Event (particle physics)","score_opus":0.017441493816929273,"score_gpt":0.22154597941610235,"score_spread":0.20410448559917307,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990377646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997687,0.00006870439,0.0002629136,0.000015452584,0.000005176303,0.000007700337,0.00029559946,0.00003869664,0.0016187415],"genre_scores_gemma":[0.9990202,0.000016271346,0.0003577915,0.000007763361,0.0000093694935,0.000003142565,0.00038150285,0.0000031250934,0.00020077385],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997931,0.000015017065,0.000009827856,0.00006114095,0.000075775046,0.000045190813],"domain_scores_gemma":[0.99933904,0.000040865478,0.0002831175,0.00006082142,0.00007765302,0.00019836733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024047178,0.00021248664,0.00020108276,0.0016789137,0.00043166548,0.00042998348,0.00030982526,0.00026874457,0.0015700952],"category_scores_gemma":[0.00072038756,0.000115245275,0.00014937848,0.00048969116,0.00020367444,0.00031436092,0.000703209,0.0002418968,0.00033778534],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019374237,0.00006945122,0.9491292,0.00001879997,0.000086937805,0.00050089834,0.00024924363,0.0003381051,0.037969448,0.00044586355,0.00042472885,0.010573577],"study_design_scores_gemma":[0.0000046505347,0.000056015622,0.99549735,0.0000021772435,0.000013557901,0.0001862059,0.000070878006,0.00080906105,0.002756915,0.00006654679,0.0005320345,0.000004675304],"about_ca_topic_score_codex":0.0034760234,"about_ca_topic_score_gemma":0.006508637,"teacher_disagreement_score":0.0034760234,"about_ca_system_score_codex":0.0005695375,"about_ca_system_score_gemma":0.0001344631,"threshold_uncertainty_score":0.006911576},"labels":[],"label_agreement":null},{"id":"W2990472889","doi":"10.3847/1538-4357/ab5ba0","title":"The Luminosity Function of Red Supergiants in M31","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Red supergiant; Astrophysics; Physics; Supergiant; Supernova; Stars; Luminosity function; Asymptotic giant branch; Galaxy; Luminosity; Initial mass function; Spiral galaxy; Astronomy; Star formation","score_opus":0.01441132662096297,"score_gpt":0.21227482392689595,"score_spread":0.19786349730593297,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990472889","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99837226,0.00005750916,0.0006060985,0.000020581596,7.957355e-7,0.0000025959075,0.00015635756,0.000028308094,0.0007554835],"genre_scores_gemma":[0.99927133,0.000014603169,0.00021270811,0.0000044586614,8.9915915e-7,0.0000021662638,0.0002853527,0.0000049635855,0.00020344791],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987376,0.000020278745,0.0000070927317,0.00003816055,0.000029444345,0.000031223706],"domain_scores_gemma":[0.99923384,0.00018745067,0.00020874872,0.00009208357,0.0001416244,0.00013626888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005290845,0.00028229313,0.00017598555,0.0012746553,0.0002549675,0.0004690422,0.00028394914,0.00038057633,0.0011853713],"category_scores_gemma":[0.0013457374,0.00010767703,0.00027191418,0.00066412915,0.00032626837,0.00031881427,0.0004530654,0.00020718398,0.0005988856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016975093,0.000025488305,0.95320874,0.000030454523,0.000031166564,0.0002270351,0.00047682977,0.004375557,0.027611338,0.0010310205,0.00037641608,0.01243611],"study_design_scores_gemma":[0.0000026436499,0.00003339808,0.9904703,0.0000041295098,0.000004730291,0.00013967787,0.000070353904,0.006447172,0.0022758597,0.00021749327,0.00032954486,0.0000047417357],"about_ca_topic_score_codex":0.005220388,"about_ca_topic_score_gemma":0.0037307115,"teacher_disagreement_score":0.005220388,"about_ca_system_score_codex":0.00061784394,"about_ca_system_score_gemma":0.00014559632,"threshold_uncertainty_score":0.01037997},"labels":[],"label_agreement":null},{"id":"W2990676792","doi":"10.3847/1538-4357/ab7e29","title":"Measurement of the Cosmic Microwave Background Polarization Lensing Power Spectrum from Two Years of POLARBEAR Data","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of California, San Diego; Office of Science; Ministry of Education, Culture, Sports, Science and Technology; European Commission; U.S. Department of Energy; McGill University; Gordon and Betty Moore Foundation; National Energy Research Scientific Computing Center; John Templeton Foundation; National Science Foundation","keywords":"Cosmic microwave background; Weak gravitational lensing; Gravitational lens; Polarization (electrochemistry); Cosmology; Observational cosmology; Dark matter; Spectral density; COSMIC cancer database","score_opus":0.027628921030337046,"score_gpt":0.2513585332218874,"score_spread":0.22372961219155035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990676792","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99498004,0.000073082185,0.0013872854,0.000049340357,0.000008064368,0.0000073491224,0.002614978,0.000099951816,0.00077989127],"genre_scores_gemma":[0.9908326,0.000054271186,0.0015137871,0.000018477402,0.000022376256,0.000012539775,0.0073495056,0.000026903876,0.0001695471],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99936765,0.00013219709,0.000036171015,0.0001446656,0.00018834474,0.00013094685],"domain_scores_gemma":[0.9972561,0.0006996896,0.00068074075,0.00049633544,0.00048770334,0.00037954023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00109687,0.00042487145,0.00045101842,0.0032486243,0.00034510414,0.0007665707,0.0003143888,0.00037399452,0.0007775709],"category_scores_gemma":[0.0021656838,0.0002797417,0.00046292561,0.0019348384,0.00030311814,0.0003872169,0.0006478652,0.00048017086,0.00028563637],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040191118,0.00018255862,0.9448537,0.000081824866,0.00041752035,0.00038202904,0.00028227278,0.0060274755,0.029324437,0.0005669494,0.0012907187,0.016188612],"study_design_scores_gemma":[0.000012673678,0.000054301763,0.9901266,0.000007982196,0.000046531306,0.00015076259,0.000063628235,0.0036259156,0.004568491,0.00010485972,0.001218148,0.000020148718],"about_ca_topic_score_codex":0.005147856,"about_ca_topic_score_gemma":0.009163962,"teacher_disagreement_score":0.005147856,"about_ca_system_score_codex":0.00036882304,"about_ca_system_score_gemma":0.00026751877,"threshold_uncertainty_score":0.010235786},"labels":[],"label_agreement":null},{"id":"W2990707837","doi":"10.3847/1538-4357/ab5d2b","title":"The Detection of Dust Gap-ring Structure in the Outer Region of the CR Cha Protoplanetary Disk","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Isotopologue; Physics; Millimeter; Submillimeter Array; Astrophysics; Planet; Protoplanetary disk; Radiative transfer; Circumstellar dust; Cosmic dust; Astronomy; Spectral line; Star formation; Stars; Optics","score_opus":0.01360723468958168,"score_gpt":0.21459332752049243,"score_spread":0.20098609283091073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2990707837","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991628,0.000054232787,0.00021556426,0.000009322643,0.000001439546,0.0000020784178,0.00006673515,0.00002263164,0.0004652881],"genre_scores_gemma":[0.99956614,0.0000110953515,0.00029533292,0.000007394143,0.0000022016375,0.0000017816554,0.000054473676,0.0000019508554,0.00005974991],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999523,0.0000032985597,0.0000015723278,0.000019007153,0.000009790633,0.000014060017],"domain_scores_gemma":[0.9998431,0.000016957878,0.000043770222,0.000019391122,0.000023078488,0.000053668202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000072321694,0.00010103036,0.00013864842,0.00042971756,0.00023698976,0.00024385702,0.00024325048,0.0002332199,0.0006919717],"category_scores_gemma":[0.00014640685,0.00012868976,0.0000885239,0.00019058879,0.00015601717,0.00013881206,0.0002218752,0.00013753577,0.00013225985],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004240822,0.00007485317,0.364479,0.000058137473,0.00005351928,0.00089753716,0.00038155625,0.0002906278,0.62128127,0.00023410084,0.00035188042,0.011473383],"study_design_scores_gemma":[0.000009494384,0.0000500032,0.9887078,0.0000029361058,0.000010101911,0.00030439036,0.00008879012,0.00090249744,0.009539325,0.00004360496,0.00033807522,0.000003133658],"about_ca_topic_score_codex":0.0013707672,"about_ca_topic_score_gemma":0.0020837311,"teacher_disagreement_score":0.0013707672,"about_ca_system_score_codex":0.00014100768,"about_ca_system_score_gemma":0.000050784678,"threshold_uncertainty_score":0.0027256012},"labels":[],"label_agreement":null},{"id":"W2991264604","doi":"10.3847/1538-4357/ab6083","title":"The NANOGrav 11 yr Data Set: Limits on Gravitational Wave Memory","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"","keywords":"Gravitational wave; Observatory; Pulsar; Amplitude; Supermassive black hole; Sky; Gravitational-wave observatory; Waveform","score_opus":0.061878327329429314,"score_gpt":0.3415050138049461,"score_spread":0.27962668647551675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2991264604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.971893,0.00019738244,0.0016443111,0.00021088419,0.000027383656,0.000027385118,0.019202845,0.000116448646,0.0066803778],"genre_scores_gemma":[0.9459006,0.000075108,0.0018733421,0.00011234934,0.00002437142,0.000038392376,0.050483376,0.00005147197,0.0014410507],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991934,0.00014641638,0.000092400565,0.00021446477,0.00027510733,0.0000781356],"domain_scores_gemma":[0.9964546,0.0015369591,0.0006512961,0.00083722867,0.00035908827,0.00016088087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013439686,0.0002773302,0.00043410528,0.0017602477,0.00034051764,0.0007933964,0.00061309634,0.00040619596,0.0020974283],"category_scores_gemma":[0.004265469,0.00013603063,0.0002955756,0.0015028758,0.0002446467,0.00064851943,0.0010064811,0.00031650538,0.0005567197],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012842948,0.00018530838,0.93010336,0.00013851757,0.00022867828,0.00047297438,0.00026383664,0.012786341,0.012314031,0.0020762524,0.010541204,0.029605098],"study_design_scores_gemma":[0.00006819352,0.00013437125,0.9469107,0.000041329997,0.000056227713,0.00031031008,0.00029552952,0.02650536,0.005146901,0.00063916796,0.019851308,0.000040610958],"about_ca_topic_score_codex":0.008434474,"about_ca_topic_score_gemma":0.016872726,"teacher_disagreement_score":0.008434474,"about_ca_system_score_codex":0.00028808851,"about_ca_system_score_gemma":0.0002068009,"threshold_uncertainty_score":0.01677078},"labels":[],"label_agreement":null},{"id":"W2991277936","doi":"10.3847/1538-4357/ab5a7e","title":"The Circumstellar Environment around the Embedded Protostar EC 53","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Astrophysics; Physics; Outflow; Circumstellar envelope; Circumstellar disk; Line (geometry); Envelope (radar); Emission spectrum; Spectral line; Astronomy; Star formation; Stars","score_opus":0.013002616010251976,"score_gpt":0.2187135174082485,"score_spread":0.2057109013979965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2991277936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986349,0.000041110325,0.00011792135,0.00000573916,8.539412e-7,0.0000013851993,0.00008447793,0.000009550632,0.0011041568],"genre_scores_gemma":[0.99962175,0.000019044135,0.00013801659,0.000004113249,7.0883095e-7,5.4301694e-7,0.00011517594,0.0000021916896,0.00009842365],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999715,0.000002518854,0.0000016987874,0.000009973203,0.00000661694,0.0000076070064],"domain_scores_gemma":[0.9999175,0.000008637399,0.000027306567,0.000011636376,0.000010577011,0.000024339388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000352026,0.0001395799,0.00012293256,0.00016080428,0.0002338654,0.00038603693,0.00011501067,0.00016103029,0.00085512135],"category_scores_gemma":[0.0001353658,0.00006995771,0.00008915418,0.000195557,0.00014504137,0.00014734309,0.00024767313,0.0001479431,0.0002683669],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030441774,0.000051330822,0.3206906,0.00003790106,0.000053061347,0.0023001798,0.00024672927,0.0019914734,0.6613135,0.00040637792,0.00035429315,0.012250147],"study_design_scores_gemma":[0.0000065113845,0.00008434458,0.98067987,0.0000058609426,0.000018994053,0.0014727209,0.00025533236,0.0024552534,0.013736049,0.000111981215,0.0011670836,0.0000059714457],"about_ca_topic_score_codex":0.0021848183,"about_ca_topic_score_gemma":0.0019361343,"teacher_disagreement_score":0.0021848183,"about_ca_system_score_codex":0.00021183568,"about_ca_system_score_gemma":0.00006815782,"threshold_uncertainty_score":0.0043441653},"labels":[],"label_agreement":null},{"id":"W2991364773","doi":"10.3847/1538-4357/ab7a27","title":"SN 2017cfd: A Normal Type Ia Supernova Discovered Very Young","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Supernova; Luminosity; Observatory; RADIUS; Extinction (optical mineralogy); Population","score_opus":0.014459658562031515,"score_gpt":0.23577879083874767,"score_spread":0.22131913227671615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2991364773","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9904156,0.0005379562,0.0011946856,0.00009375454,0.00010186203,0.000052795003,0.0030179576,0.00010838422,0.0044769445],"genre_scores_gemma":[0.99448144,0.0001723116,0.00071737403,0.00007059963,0.000040168947,0.000018508112,0.0034855716,0.000020560343,0.0009933552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997329,0.000011324302,0.00002684869,0.00007553765,0.000075888296,0.00007746761],"domain_scores_gemma":[0.9989195,0.00011331789,0.00021070884,0.00013024836,0.00021113871,0.00041516623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037209596,0.0004368315,0.00059042894,0.0016447542,0.0007297359,0.0008820868,0.00030789833,0.00038072257,0.0017130068],"category_scores_gemma":[0.00096332055,0.00012983284,0.00036047903,0.0007359788,0.0005516226,0.00026721542,0.00085091393,0.0004322712,0.0005597653],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024791516,0.00007090314,0.96192044,0.00007551192,0.0000784185,0.0083046565,0.00012739701,0.00022246827,0.0068081818,0.0013101435,0.0025367222,0.018297242],"study_design_scores_gemma":[0.00002236061,0.00018374779,0.94100773,0.00006549224,0.000051764076,0.030596912,0.00038507144,0.000922274,0.004862176,0.0012153329,0.020660512,0.000026553122],"about_ca_topic_score_codex":0.0062935036,"about_ca_topic_score_gemma":0.008773932,"teacher_disagreement_score":0.0062935036,"about_ca_system_score_codex":0.00079470506,"about_ca_system_score_gemma":0.0006103639,"threshold_uncertainty_score":0.012513757},"labels":[],"label_agreement":null},{"id":"W2991544253","doi":"10.3847/1538-4357/abe62f","title":"PINT: A Modern Software Package for Pulsar Timing","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":168,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Pulsar; Software; Suite; Static timing analysis; Software package; Code (set theory); Software suite; Object-oriented programming","score_opus":0.02322213065659653,"score_gpt":0.3285783299775095,"score_spread":0.305356199320913,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2991544253","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0026777089,0.0002597782,0.41925958,0.00021513768,0.00049734843,0.0003287489,0.029578006,0.5411577,0.0060260114],"genre_scores_gemma":[0.04741962,0.0006639386,0.4962322,0.00097310444,0.00041949202,0.0035461541,0.099843875,0.3380334,0.0128682265],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9981194,0.0002533461,0.00027769964,0.0003904671,0.00076079875,0.0001982704],"domain_scores_gemma":[0.9973073,0.0008958417,0.00043278924,0.00045955073,0.0007118069,0.00019273785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029166916,0.0018607271,0.001238014,0.0020209884,0.0008477895,0.0020107632,0.00307113,0.00080364663,0.05186183],"category_scores_gemma":[0.009830423,0.0012987537,0.0019714762,0.0022289653,0.0007533105,0.002537676,0.003111001,0.0035452344,0.03235025],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094782305,0.0001440085,0.0053007537,0.0028745367,0.0005042424,0.00057019404,0.0006657511,0.018486448,0.021649022,0.018754026,0.67456573,0.2555375],"study_design_scores_gemma":[0.00041128328,0.0002028074,0.005806098,0.00035636482,0.00019104574,0.0007887851,0.00008156369,0.10130801,0.043104693,0.033660386,0.813708,0.00038081987],"about_ca_topic_score_codex":0.0017783409,"about_ca_topic_score_gemma":0.0012004972,"teacher_disagreement_score":0.05186183,"about_ca_system_score_codex":0.00061966054,"about_ca_system_score_gemma":0.0028674272,"threshold_uncertainty_score":0.17349505},"labels":[],"label_agreement":null},{"id":"W2991972750","doi":"10.3847/1538-4357/ab9b29","title":"Global 21 cm Signal Extraction from Foreground and Instrumental Effects. II. Efficient and Self-consistent Technique for Constraining Nonlinear Signal Models","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Markov chain Monte Carlo; SIGNAL (programming language); Prior probability; Pipeline (software); Monte Carlo method; Nonlinear system; Pattern recognition (psychology); Parameter space","score_opus":0.012616248567348401,"score_gpt":0.22991622930268252,"score_spread":0.21729998073533413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2991972750","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.12712385,0.00010732011,0.87010264,0.00010017417,0.000008541619,0.000040102866,0.00022548003,0.0009797151,0.001312244],"genre_scores_gemma":[0.5775148,0.00013324828,0.41920727,0.000059188817,0.000017449956,0.00009368733,0.00093465,0.00040153545,0.0016381723],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998264,0.000035683915,0.000007804753,0.000043857275,0.0000644961,0.000021946704],"domain_scores_gemma":[0.99960595,0.0001277193,0.000074982054,0.00012437388,0.000043711836,0.000023240853],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007076214,0.000797613,0.00040775072,0.000731678,0.0003267574,0.00062938925,0.0007211534,0.00046409338,0.001376049],"category_scores_gemma":[0.0015058181,0.0005327579,0.0007744392,0.00061808625,0.0005068262,0.0007296132,0.0010982063,0.00086321624,0.0005559431],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034823056,0.00012439227,0.02590138,0.00020302658,0.00020278704,0.0001990433,0.00028878637,0.2812089,0.22675903,0.018045628,0.0012343092,0.44548446],"study_design_scores_gemma":[0.000017856688,0.0000550168,0.009270664,0.000011700578,0.000036125453,0.000070209026,0.000037514154,0.93315995,0.046327986,0.009103912,0.0018764504,0.000032590808],"about_ca_topic_score_codex":0.0017100697,"about_ca_topic_score_gemma":0.004408535,"teacher_disagreement_score":0.0017100697,"about_ca_system_score_codex":0.00038579982,"about_ca_system_score_gemma":0.00078262016,"threshold_uncertainty_score":0.004603386},"labels":[],"label_agreement":null},{"id":"W2992033556","doi":"10.3847/1538-4357/ab5db5","title":"GS 2000+25: The Least Luminous Black Hole X-Ray Binary","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Jansky; Black hole (networking); Binary black hole; Luminosity; Intermediate-mass black hole; Eddington luminosity; Spin-flip","score_opus":0.017838870707925107,"score_gpt":0.22275637694492106,"score_spread":0.20491750623699595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2992033556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99841046,0.00011486668,0.000060174098,0.000012422271,0.000002449692,0.0000027381561,0.0001385262,0.00001758434,0.0012407973],"genre_scores_gemma":[0.9991592,0.000021823107,0.00009352392,0.000010999814,0.0000033913832,6.941536e-7,0.0002951643,0.0000023385137,0.00041293507],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999455,0.0000043565447,0.0000031484233,0.000017669703,0.000010643179,0.000018706834],"domain_scores_gemma":[0.9998362,0.000009253141,0.000047152134,0.000013100431,0.000009929387,0.000084262836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009739557,0.000230374,0.00022893409,0.0007024927,0.0003268627,0.0005991903,0.00019125396,0.000157303,0.002131933],"category_scores_gemma":[0.00021164166,0.000061358165,0.00007726324,0.00038428532,0.00026138962,0.00017721021,0.00028822423,0.00010028352,0.00049962173],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090583554,0.00013648215,0.8966337,0.00007457082,0.00007659898,0.00096915464,0.0005736788,0.0005042585,0.065812506,0.0016067646,0.0012552197,0.031451363],"study_design_scores_gemma":[0.000028843056,0.00022877277,0.98810726,0.000011092969,0.000026559715,0.0012197875,0.00024159533,0.0004240371,0.005067206,0.00051688397,0.004119554,0.000008435955],"about_ca_topic_score_codex":0.0023812233,"about_ca_topic_score_gemma":0.0028411478,"teacher_disagreement_score":0.0023812233,"about_ca_system_score_codex":0.00023378182,"about_ca_system_score_gemma":0.0001036513,"threshold_uncertainty_score":0.0071320534},"labels":[],"label_agreement":null},{"id":"W2992394350","doi":"10.3847/1538-4357/ab5db6","title":"Substructure of Visibility Functions from Scattered Radio Emission of Pulsars through Space VLBI","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Pulsar; Scattering; Visibility; Substructure; Radio telescope; Very-long-baseline interferometry; LOFAR; Scintillation; Interstellar medium","score_opus":0.014400580127016071,"score_gpt":0.23070820772573508,"score_spread":0.21630762759871902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2992394350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965599,0.00009903521,0.0021801519,0.000020762194,0.000005519459,0.0000045444203,0.0003360776,0.00014570857,0.00064828456],"genre_scores_gemma":[0.99826694,0.000020858859,0.000604485,0.0000060799143,0.000005596451,0.0000041504973,0.00094399415,0.000044673867,0.000103135964],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973696,0.000027099482,0.00001391766,0.000061599516,0.000091272814,0.00006904828],"domain_scores_gemma":[0.997733,0.00074463943,0.0005028692,0.00036616088,0.00040837034,0.00024496953],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052303233,0.0002927824,0.00033505898,0.002951124,0.0002704044,0.0007672481,0.0003930233,0.0004098907,0.00046741802],"category_scores_gemma":[0.00300791,0.00029688972,0.0005323239,0.0012731574,0.00032487907,0.00036882074,0.0005744034,0.0004607135,0.00018657216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010314812,0.00013210716,0.72433174,0.00009660854,0.00051999505,0.000573059,0.0013386423,0.012599151,0.21103844,0.0011403668,0.0008709757,0.046327405],"study_design_scores_gemma":[0.000006511316,0.0000394112,0.9869876,0.000006280003,0.000024370918,0.00017566132,0.000067648914,0.0083220145,0.0038024385,0.0001603607,0.00039219548,0.000015616408],"about_ca_topic_score_codex":0.0027593093,"about_ca_topic_score_gemma":0.0021929585,"teacher_disagreement_score":0.002951124,"about_ca_system_score_codex":0.0004215347,"about_ca_system_score_gemma":0.00014581486,"threshold_uncertainty_score":0.005486548},"labels":[],"label_agreement":null},{"id":"W2992477749","doi":"10.3847/1538-4357/ab5fd9","title":"The Colors and Sizes of Recently Quenched Galaxies: A Result of Compact Starburst before Quenching","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council; East Asian Core Observatories Association; European Commission","keywords":"Galaxy; Star formation; Balmer series; Peculiar galaxy; Gravitational collapse; Galaxy merger; Galaxy formation and evolution; Quenching (fluorescence)","score_opus":0.009926965433212,"score_gpt":0.22127042213935313,"score_spread":0.21134345670614113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2992477749","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996971,0.00004435544,0.00007430901,0.000011496508,7.642452e-7,0.0000010349878,0.000057921505,0.000006666645,0.000106442145],"genre_scores_gemma":[0.9998171,0.0000069354132,0.00002687234,0.0000058547134,0.0000018917306,5.468287e-7,0.000102969294,0.000001691582,0.000036213383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999818,0.000030263272,0.0000111432,0.0000592984,0.000039662173,0.000041651667],"domain_scores_gemma":[0.9975949,0.0005105729,0.0009665797,0.00026541352,0.00016547399,0.00049711217],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040396437,0.00017298639,0.00026230558,0.0007836318,0.00018876686,0.0005724028,0.00048606214,0.00033780726,0.00086363417],"category_scores_gemma":[0.0017469125,0.00018185264,0.00030288764,0.0004780739,0.00051830173,0.0002551341,0.00033881338,0.00029762145,0.00016913717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015978944,0.000024482759,0.9868427,0.000006550336,0.000042771724,0.0002925555,0.00018036993,0.00034769817,0.010190663,0.00009337465,0.000056937202,0.0017621049],"study_design_scores_gemma":[0.0000038809735,0.000030243986,0.99869305,0.000001114491,0.00000986933,0.00018678351,0.00004115336,0.0005459603,0.00037429918,0.000041988496,0.00006909738,0.0000025899228],"about_ca_topic_score_codex":0.0031189453,"about_ca_topic_score_gemma":0.0025328756,"teacher_disagreement_score":0.0031189453,"about_ca_system_score_codex":0.0004398769,"about_ca_system_score_gemma":0.000075299824,"threshold_uncertainty_score":0.0062015653},"labels":[],"label_agreement":null},{"id":"W2992842848","doi":"10.3847/1538-4357/ab1b15","title":"Constraining the Neutron Star Radius with Joint Gravitational-wave and Short Gamma-Ray Burst Observations of Neutron Star–Black Hole Coalescing Binaries","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Neutron star; Gravitational wave; RADIUS; Torus; Accretion (finance); Gamma-ray burst; Binary number; Accretion disc; Coalescence (physics)","score_opus":0.031038073604297913,"score_gpt":0.27796145709910597,"score_spread":0.24692338349480805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2992842848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.985494,0.00027812284,0.012349239,0.000029135697,0.000013673897,0.000011908492,0.00019590234,0.00011004835,0.0015179728],"genre_scores_gemma":[0.99517596,0.00003795815,0.004447006,0.0000069942776,0.0000102454715,0.0000057883653,0.00017631326,0.0000116119645,0.00012810643],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99949706,0.00013575435,0.00003731237,0.00012630296,0.00015000477,0.000053593987],"domain_scores_gemma":[0.99813914,0.00043014745,0.00062417844,0.00035625004,0.00019724645,0.00025294046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015021724,0.0004091696,0.00040622652,0.0012198433,0.00034014776,0.0010364036,0.0004189045,0.00040714926,0.0005290817],"category_scores_gemma":[0.0031968593,0.0003631505,0.00034591721,0.0006493163,0.00039697537,0.0007316637,0.0016885567,0.00035820933,0.00025374262],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006969227,0.00009970132,0.8275374,0.000052948493,0.00029596695,0.00024049326,0.00029275718,0.010773428,0.133637,0.0023602564,0.00029137926,0.023721742],"study_design_scores_gemma":[0.000049975035,0.00021364643,0.8230414,0.0000331175,0.00015249151,0.00049675396,0.00016111061,0.12511657,0.046083797,0.0021873806,0.0024069494,0.000056832345],"about_ca_topic_score_codex":0.0021142673,"about_ca_topic_score_gemma":0.003618636,"teacher_disagreement_score":0.0021142673,"about_ca_system_score_codex":0.00027033634,"about_ca_system_score_gemma":0.00022990005,"threshold_uncertainty_score":0.0079443455},"labels":[],"label_agreement":null},{"id":"W2992863588","doi":"10.3847/1538-4357/ab5e85","title":"Discovery of Protoclusters at z ∼ 3.7 and 4.9: Embedded in Primordial Superclusters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Japan Society for the Promotion of Science; Science and Technology Facilities Council","keywords":"Redshift; Galaxy; Velocity dispersion; William Herschel Telescope; Telescope; Halo; Galaxy cluster","score_opus":0.008562654905404112,"score_gpt":0.21124196244615132,"score_spread":0.2026793075407472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2992863588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986979,0.00013711731,0.00053372997,0.000016391421,0.0000028080926,0.0000050073795,0.0001543823,0.00003722285,0.00041542496],"genre_scores_gemma":[0.9989945,0.000036172616,0.00056596234,0.000012236648,0.0000035052467,0.0000020884088,0.00021730746,0.0000047446615,0.00016355819],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999895,0.000005267575,0.0000035579435,0.000028005312,0.000032719985,0.000035409696],"domain_scores_gemma":[0.99928623,0.00006979268,0.00026927178,0.000079190606,0.00010459532,0.00019102843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001683926,0.00017432928,0.00018053957,0.00090437866,0.00035530937,0.0004947786,0.0003005937,0.00017442471,0.0009565581],"category_scores_gemma":[0.00039843083,0.000182019,0.00019196556,0.0004464758,0.00037694175,0.00025121888,0.00044653623,0.00026361205,0.00023041708],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009728709,0.000019106972,0.9168139,0.000019917547,0.00004738786,0.0004317371,0.00028033985,0.00015417581,0.0768948,0.00026349458,0.00021720723,0.004760658],"study_design_scores_gemma":[0.0000021651897,0.000015881486,0.9948667,0.0000020190812,0.000010570013,0.00019148391,0.00007086014,0.0003199854,0.0039675822,0.00008573186,0.0004629576,0.000003946013],"about_ca_topic_score_codex":0.0033985288,"about_ca_topic_score_gemma":0.0046964437,"teacher_disagreement_score":0.0033985288,"about_ca_system_score_codex":0.0003128761,"about_ca_system_score_gemma":0.000088950714,"threshold_uncertainty_score":0.006757498},"labels":[],"label_agreement":null},{"id":"W2993625252","doi":"10.3847/1538-4357/ab6221","title":"The CO(3–2)/CO(1–0) Luminosity Line Ratio in Nearby Star-forming Galaxies and Active Galactic Nuclei from xCOLD GASS, BASS, and SLUGS","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Science and Technology Facilities Council","keywords":"Active galactic nucleus; Galaxy; Luminosity; Star formation; Interstellar medium; Line (geometry); Universe; Luminous infrared galaxy","score_opus":0.0102026039835137,"score_gpt":0.2187455318647481,"score_spread":0.2085429278812344,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2993625252","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997899,0.000023673327,0.0000101438945,0.0000029630273,4.0280554e-7,5.6314695e-7,0.00007106412,0.0000016648047,0.00009974963],"genre_scores_gemma":[0.9996996,0.000010227338,0.000016757684,0.0000023476755,9.528823e-7,6.907303e-7,0.00020159692,7.700694e-7,0.00006703552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998734,0.000018670267,0.0000083765235,0.000039778468,0.000025262076,0.000034546323],"domain_scores_gemma":[0.99941957,0.00007215799,0.00017374437,0.00004331245,0.00006799762,0.00022322562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032583415,0.00022702389,0.0002477423,0.0015339917,0.0002974473,0.00043129487,0.00026031645,0.00019709536,0.0013487398],"category_scores_gemma":[0.00059016846,0.00014507733,0.00019270225,0.00043115224,0.00052848796,0.00024729347,0.00033876346,0.00015010481,0.00025244174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008311506,0.000010354717,0.9977443,0.0000027194353,0.000016270491,0.00004876507,0.0001342659,0.00004392019,0.0011954891,0.000024987125,0.00003486658,0.0006609687],"study_design_scores_gemma":[0.0000020000584,0.000020368056,0.9993789,0.0000016200738,0.000005678353,0.00006337661,0.00016352502,0.00013283553,0.00017234137,0.0000098995215,0.000048102407,0.0000011891581],"about_ca_topic_score_codex":0.023181895,"about_ca_topic_score_gemma":0.027692562,"teacher_disagreement_score":0.023181895,"about_ca_system_score_codex":0.00036302584,"about_ca_system_score_gemma":0.00012586678,"threshold_uncertainty_score":0.04609388},"labels":[],"label_agreement":null},{"id":"W2994013726","doi":"10.3847/1538-4357/ab71ff","title":"Saturn’s Probable Interior: An Exploration of Saturn’s Potential Interior Density Structures","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"National Aeronautics and Space Administration","keywords":"Density contrast; RADIUS; Markov chain Monte Carlo; Gravitation; Monte Carlo method; Gravitational field; Field (mathematics); Inner core; Gravitational potential","score_opus":0.01900863397439669,"score_gpt":0.23065897375813169,"score_spread":0.211650339783735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2994013726","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9647443,0.0004039004,0.028030297,0.00061909633,0.000004705203,0.000013699433,0.000526753,0.00010314857,0.005554158],"genre_scores_gemma":[0.9912778,0.00012766111,0.007758398,0.000029626202,0.000011788356,0.0000066670495,0.0003592922,0.00004980285,0.0003789448],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998764,0.00005463524,0.0000027476501,0.000023948445,0.000024159142,0.000018142466],"domain_scores_gemma":[0.9987575,0.00091587467,0.00008384001,0.00006199084,0.00008405192,0.000096768716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001082425,0.00018099617,0.0003649592,0.0010610162,0.00065472967,0.0010118112,0.00054960646,0.00042965083,0.0024100086],"category_scores_gemma":[0.003978578,0.00029451653,0.00045239602,0.00062123826,0.0007480012,0.00074383826,0.0010809524,0.0005765804,0.0001189875],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003501429,0.00006923028,0.17159027,0.00018725844,0.00023983202,0.0008224366,0.0022681765,0.7202671,0.0053963233,0.0706735,0.0029704387,0.025165377],"study_design_scores_gemma":[0.000026879481,0.00003613747,0.048365045,0.00004390037,0.000029466964,0.00013270503,0.0006775159,0.90820074,0.0008206462,0.039061066,0.0025666372,0.000039222406],"about_ca_topic_score_codex":0.024238186,"about_ca_topic_score_gemma":0.02308086,"teacher_disagreement_score":0.024238186,"about_ca_system_score_codex":0.0014869014,"about_ca_system_score_gemma":0.0007192358,"threshold_uncertainty_score":0.04819423},"labels":[],"label_agreement":null},{"id":"W2994141210","doi":"10.3847/1538-4357/abab99","title":"Constraining Galactic Structure with the LISA White Dwarf Foreground","year":2020,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; White dwarf; Astrophysics; Population; Milky Way; Astronomy; Galaxy; Dwarf galaxy; Stars","score_opus":0.01655441947699467,"score_gpt":0.23018141236422662,"score_spread":0.21362699288723194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2994141210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9794078,0.00015231609,0.015959827,0.000057861093,0.000006718341,0.0000066163784,0.0005701274,0.00019699814,0.0036416503],"genre_scores_gemma":[0.9944905,0.000026643844,0.0048552942,0.000011247229,0.000008402867,0.0000033426436,0.00036761473,0.000025828951,0.00021106654],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998722,0.000028360115,0.000004346175,0.000047459984,0.00002905545,0.00001853621],"domain_scores_gemma":[0.9994691,0.00022811534,0.000099554294,0.00008523073,0.00005608689,0.00006186226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005264349,0.00029873184,0.00022336651,0.001218025,0.0003077108,0.0010164169,0.00021778414,0.00022674374,0.0012375083],"category_scores_gemma":[0.0011333595,0.00022498328,0.0002793089,0.00069775176,0.00022181087,0.00035404883,0.0005416973,0.0001891847,0.00033973326],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003405103,0.00009962625,0.78800046,0.00006419276,0.00021512374,0.0001643758,0.00025111402,0.038331274,0.10412026,0.009099055,0.00075649,0.05855755],"study_design_scores_gemma":[0.000033097316,0.00007909705,0.68529886,0.000024274905,0.000089535235,0.00015310642,0.00017655647,0.2762918,0.027294237,0.006540201,0.0039926604,0.000026582216],"about_ca_topic_score_codex":0.0034534447,"about_ca_topic_score_gemma":0.004385923,"teacher_disagreement_score":0.0034534447,"about_ca_system_score_codex":0.0004983378,"about_ca_system_score_gemma":0.00018746483,"threshold_uncertainty_score":0.0068666935},"labels":[],"label_agreement":null},{"id":"W2995071660","doi":"10.3847/1538-4357/ab07be","title":"Results from EDGES High-Band. III. New Constraints on Parameters of the Early Universe","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Reionization; Cosmic microwave background; Quasar; Optical depth; Halo; Spectral line; Radiative transfer; Photon; Cosmic background radiation; Background radiation","score_opus":0.008433826791812584,"score_gpt":0.1910460759928442,"score_spread":0.1826122492010316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995071660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9459806,0.0006232073,0.027196927,0.00021151977,0.000022835424,0.00001615532,0.006690679,0.00042449264,0.018833505],"genre_scores_gemma":[0.98806596,0.0001090991,0.005640228,0.000059645838,0.000013459041,0.000007968243,0.004137418,0.00009504618,0.0018712617],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996538,0.00009364012,0.000015212451,0.00009196918,0.00009514585,0.000050186467],"domain_scores_gemma":[0.9984353,0.00062604295,0.00019567211,0.0004202206,0.00022828615,0.00009446505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009338537,0.00058680255,0.00027128987,0.0007511936,0.000190831,0.0008296275,0.00030199662,0.0003931438,0.005373962],"category_scores_gemma":[0.0021372654,0.00014409791,0.00057915226,0.0004939564,0.00017651677,0.00059849303,0.00061844755,0.00034278035,0.0009636442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026350182,0.00025466285,0.46037853,0.00050941686,0.0011201684,0.00044554542,0.00030697824,0.26127064,0.07009444,0.008984691,0.0072268313,0.18677308],"study_design_scores_gemma":[0.00007915219,0.0002630723,0.7059029,0.00010562409,0.00035641814,0.00041524981,0.00033479766,0.1886541,0.07382324,0.00866503,0.021308547,0.00009192695],"about_ca_topic_score_codex":0.0037224016,"about_ca_topic_score_gemma":0.0038526633,"teacher_disagreement_score":0.005373962,"about_ca_system_score_codex":0.00030012292,"about_ca_system_score_gemma":0.000127924,"threshold_uncertainty_score":0.017977655},"labels":[],"label_agreement":null},{"id":"W2995187834","doi":"10.3847/1538-4357/ab12dd","title":"Bright Mini-outburst Ends the 12 yr Long Activity of the Black Hole Candidate Swift J1753.5–0127","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Goddard Space Flight Center; National Aeronautics and Space Administration","keywords":"Extrapolation; Black hole (networking); Flux (metallurgy); Orbital period; Swift; X-ray binary; Light curve; Optical depth","score_opus":0.009099124582273233,"score_gpt":0.22088881596641644,"score_spread":0.2117896913841432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995187834","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993414,0.00006445577,0.00009690927,0.000010678869,0.000005527301,0.0000028802922,0.00014401166,0.0000108315935,0.00032333852],"genre_scores_gemma":[0.9991596,0.000021003003,0.00012768016,0.00000972852,0.000009459052,0.0000031088757,0.00043251846,0.0000036662684,0.00023331196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999591,0.0000022421407,0.0000017616177,0.000010586735,0.000009065752,0.00001717915],"domain_scores_gemma":[0.9998154,0.000009418734,0.00006912215,0.000012479128,0.000023091101,0.0000704739],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001057188,0.00017445249,0.00017609885,0.00054888014,0.0003112787,0.00028657063,0.00016249125,0.0001500566,0.00077474915],"category_scores_gemma":[0.00018953516,0.000066851666,0.00014112605,0.00023324725,0.00015358289,0.00015029745,0.00026303812,0.00018381875,0.00020311939],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045175996,0.00010039536,0.8851466,0.000041436197,0.000051666186,0.0021238613,0.0004135937,0.00034610098,0.096818976,0.0002795046,0.0013286589,0.012897426],"study_design_scores_gemma":[0.0000030298124,0.00006274802,0.9964933,0.0000031595628,0.000007336066,0.00031917106,0.00008469815,0.0003245902,0.0020019824,0.000029294804,0.0006672784,0.0000035289684],"about_ca_topic_score_codex":0.0019984657,"about_ca_topic_score_gemma":0.00454086,"teacher_disagreement_score":0.0019984657,"about_ca_system_score_codex":0.00015056627,"about_ca_system_score_gemma":0.00008644094,"threshold_uncertainty_score":0.0039737225},"labels":[],"label_agreement":null},{"id":"W2995417213","doi":"10.3847/1538-4357/ab6328","title":"Flash Ionization Signatures in the Type Ibn Supernova SN 2019uo","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Supernova; Light curve; Luminosity; Ionization; Spectral line; Line (geometry); Type (biology)","score_opus":0.01385105756511413,"score_gpt":0.23151307241534277,"score_spread":0.21766201485022865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995417213","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980709,0.00011442719,0.00008275425,0.0000062819995,0.000007046935,0.0000033436136,0.0003020784,0.0000097960055,0.0014034541],"genre_scores_gemma":[0.99884677,0.00004235542,0.00007126571,0.000007838821,0.0000032904381,0.0000024211297,0.0006341458,0.0000019876884,0.00038984435],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999665,0.0000022048562,0.0000023978178,0.00001063417,0.000007945568,0.000010328315],"domain_scores_gemma":[0.9999058,0.000007655929,0.000030371784,0.0000070279416,0.000013738538,0.000035346886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007741221,0.00021309631,0.00018296401,0.0004912716,0.00025878617,0.00032089124,0.00012617356,0.00015901316,0.0010774204],"category_scores_gemma":[0.00014156166,0.00007986973,0.00012451876,0.0002825441,0.00012007177,0.00008898405,0.0003026264,0.00011090733,0.00020966788],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072683935,0.00012428839,0.8740763,0.000053113876,0.000055785833,0.0022359611,0.00013848298,0.00045235077,0.10845609,0.00046138326,0.0005581345,0.012661364],"study_design_scores_gemma":[0.0000037846912,0.000108611035,0.9937109,0.0000059626673,0.000008558453,0.0011699565,0.00009711016,0.00047306975,0.0029802239,0.0000834841,0.0013533281,0.000005084415],"about_ca_topic_score_codex":0.0033692215,"about_ca_topic_score_gemma":0.00599062,"teacher_disagreement_score":0.0033692215,"about_ca_system_score_codex":0.00024117898,"about_ca_system_score_gemma":0.0000629746,"threshold_uncertainty_score":0.0066992044},"labels":[],"label_agreement":null},{"id":"W2995448385","doi":"10.3847/1538-4357/ab4196","title":"[C i](1–0) and [C i](2–1) in Resolved Local Galaxies*","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia; McMaster University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Galaxy; Line (geometry); H-alpha; Interstellar medium; Emission spectrum; Spectral line; Astronomy","score_opus":0.006723787783881619,"score_gpt":0.2201034133314748,"score_spread":0.21337962554759318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995448385","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992964,0.000062370986,0.00018421425,0.0000054885395,5.344528e-7,0.0000018257631,0.000040424762,0.000016739667,0.0003920358],"genre_scores_gemma":[0.99973327,0.000010527848,0.00012887683,0.000003838916,0.000001301027,0.0000013402514,0.00006680267,0.0000040982013,0.000049955648],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983704,0.000014428294,0.0000043065625,0.00008049015,0.000023165381,0.00004060064],"domain_scores_gemma":[0.9992448,0.00013862253,0.00024095176,0.00008128753,0.00010183836,0.00019250863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037979058,0.0003128233,0.00026185383,0.0009463374,0.00033550584,0.00068194664,0.00044903177,0.0003961875,0.00082197227],"category_scores_gemma":[0.00095004943,0.00031228786,0.0002582801,0.00064542744,0.0005189365,0.0003347525,0.0003496317,0.00026816383,0.0001897411],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035919074,0.00010119177,0.9222699,0.000037580114,0.0001924033,0.00021545126,0.00068981363,0.005603029,0.06364511,0.00054857455,0.0001880178,0.006149872],"study_design_scores_gemma":[0.000010503425,0.00004813565,0.9910273,0.000004226638,0.000038111022,0.00005108171,0.00013247225,0.0051032975,0.0032435828,0.00010341478,0.00022828049,0.0000097097645],"about_ca_topic_score_codex":0.010792792,"about_ca_topic_score_gemma":0.009464675,"teacher_disagreement_score":0.010792792,"about_ca_system_score_codex":0.0007393182,"about_ca_system_score_gemma":0.00010715831,"threshold_uncertainty_score":0.021459937},"labels":[],"label_agreement":null},{"id":"W2995780368","doi":"10.3847/1538-4357/ab4e95","title":"Probing Coronal Magnetic Fields with Sungrazing Comets: H i Lyα from Pickup Ions","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Solar wind; Comet; Plasma; Population; Comet tail; Spectral line; Magnetic field; Solar radius; Doppler effect; Redshift","score_opus":0.0057206256817026275,"score_gpt":0.188161180872999,"score_spread":0.18244055519129637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995780368","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935121,0.00006950504,0.0028532909,0.00018153628,0.000014415444,0.00002543702,0.00021488937,0.00015667893,0.0029721921],"genre_scores_gemma":[0.9983551,0.000032234126,0.0012036327,0.000029212622,0.00000650633,0.000009464912,0.0001234976,0.000013351332,0.00022690781],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.999915,0.00001567497,0.0000043806003,0.000017335758,0.000022149568,0.000025438623],"domain_scores_gemma":[0.9995828,0.00018144555,0.000061261904,0.000033860346,0.000045321474,0.00009538266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003546642,0.00036681382,0.0005177344,0.0002884117,0.00068751496,0.000733826,0.0010345357,0.000984808,0.0025371427],"category_scores_gemma":[0.0010815792,0.00028538622,0.00067402766,0.00031110365,0.0005362897,0.000539612,0.00051469606,0.00052512967,0.00018048192],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002602466,0.00020718492,0.049620815,0.00006599816,0.00014424167,0.0005751735,0.0002674328,0.92495954,0.019171216,0.0012716234,0.00044442358,0.003012115],"study_design_scores_gemma":[0.000114440736,0.00015863209,0.014283746,0.000005935598,0.000029147244,0.000066915025,0.00009830874,0.9798855,0.0045477734,0.00048210923,0.0003057337,0.000021722039],"about_ca_topic_score_codex":0.023819935,"about_ca_topic_score_gemma":0.010789686,"teacher_disagreement_score":0.023819935,"about_ca_system_score_codex":0.001692322,"about_ca_system_score_gemma":0.0005022235,"threshold_uncertainty_score":0.047362566},"labels":[],"label_agreement":null},{"id":"W2995802805","doi":"10.3847/1538-4357/ab62ad","title":"Metallicity and α-Element Abundance Gradients along the Sagittarius Stream as Seen by APOGEE","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leverhulme Trust; Ministerio de Ciencia, Innovación y Universidades; Universidad Nacional Autónoma de México; Magyar Tudományos Akadémia; Space Telescope Science Institute; University of Hull; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Leibniz-Gemeinschaft; University of Notre Dame; European Regional Development Fund; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Yale University","keywords":"Metallicity; Milky Way; Sagittarius; Stars; Context (archaeology); Giant star","score_opus":0.011007421856092785,"score_gpt":0.22063062148761503,"score_spread":0.20962319963152223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995802805","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99971944,0.000010584662,0.000016710603,0.0000066622306,4.3908742e-7,5.3340887e-7,0.000073801464,0.0000028017396,0.00016902704],"genre_scores_gemma":[0.9996251,0.00001349742,0.00003946686,0.0000052654705,0.0000012341047,6.11186e-7,0.00019873868,0.0000016643,0.000114395276],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999434,0.000008527454,0.000004545426,0.00001940972,0.000011660384,0.000012467735],"domain_scores_gemma":[0.9996706,0.000032542193,0.00013457015,0.000022350338,0.00004574586,0.0000942149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000116377865,0.00012592944,0.00016967054,0.0008040001,0.0001919385,0.00045506662,0.0001298711,0.00017216316,0.0007727981],"category_scores_gemma":[0.00041552723,0.00008380227,0.00011969635,0.00047886337,0.00025850724,0.0001905706,0.0003634629,0.00012201473,0.0002402364],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005625366,0.0000077247905,0.9951874,0.0000019097615,0.000013401027,0.00005822962,0.00013045907,0.00004789911,0.003188904,0.0000301016,0.00005062929,0.0012270226],"study_design_scores_gemma":[6.328741e-7,0.000013150533,0.99962986,5.4818815e-7,0.0000018392665,0.000038448004,0.00006953766,0.00007569876,0.00010057429,0.000010918198,0.000058056583,6.972113e-7],"about_ca_topic_score_codex":0.007535168,"about_ca_topic_score_gemma":0.011764026,"teacher_disagreement_score":0.007535168,"about_ca_system_score_codex":0.0002414887,"about_ca_system_score_gemma":0.00008952486,"threshold_uncertainty_score":0.014982581},"labels":[],"label_agreement":null},{"id":"W2995874836","doi":"10.3847/1538-4357/ab4e99","title":"Tying Spatial Variations in Polycyclic Aromatic Hydrocarbon (PAH) Emission to a Changing PAH Population in the Reflection Nebula NGC 2023","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Aeronautics and Space Administration","keywords":"Physics; Reflection nebula; Polycyclic aromatic hydrocarbon; Astrophysics; Nebula; Reflection (computer programming); Astronomy; Population; Astrobiology; Stars","score_opus":0.011010684406072325,"score_gpt":0.25984663563116767,"score_spread":0.24883595122509533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995874836","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988226,0.000017855546,0.0007135846,0.0000054792813,7.406121e-7,0.0000031824743,0.00010300528,0.000056189012,0.00027732554],"genre_scores_gemma":[0.999054,0.0000075925145,0.0006167225,0.0000037521995,9.536484e-7,0.0000030449826,0.00023157761,0.000010286671,0.00007203482],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999379,0.0000062775243,0.0000027260378,0.000024739715,0.000016448423,0.00001189529],"domain_scores_gemma":[0.9998337,0.000024154679,0.000043464825,0.000028013852,0.000040329254,0.000030277317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015655169,0.00015286611,0.0001264378,0.00067878247,0.00017563753,0.00024633124,0.0002414544,0.000210011,0.00053961645],"category_scores_gemma":[0.0003164019,0.00010803648,0.00023590673,0.00036464553,0.0001324546,0.00017391687,0.00016253961,0.00013358818,0.0002587304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002844389,0.00010025177,0.62051684,0.000028648667,0.00008656645,0.00027570775,0.0002138015,0.0051235883,0.35328454,0.00015752784,0.00021167882,0.019716436],"study_design_scores_gemma":[0.0000024439717,0.000029818933,0.98416257,0.0000011085799,0.000009543373,0.00011818264,0.000080388905,0.007039185,0.008386612,0.000033256954,0.00013260527,0.0000043690993],"about_ca_topic_score_codex":0.0055465205,"about_ca_topic_score_gemma":0.0066423523,"teacher_disagreement_score":0.0055465205,"about_ca_system_score_codex":0.00026992452,"about_ca_system_score_gemma":0.00012094993,"threshold_uncertainty_score":0.011028469},"labels":[],"label_agreement":null},{"id":"W2995991094","doi":"10.3847/1538-4357/ab643e","title":"The GBT Diffuse Ionized Gas Survey: Tracing the Diffuse Ionized Gas around the Giant Hii Region W43","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Galaxy; Ionization; Line (geometry); Plasma; Spectral line; Atomic physics; Ion; Astronomy; Geometry; Nuclear physics","score_opus":0.02567171356469787,"score_gpt":0.24097184231734073,"score_spread":0.21530012875264287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2995991094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99787796,0.00010101489,0.00034644303,0.000040133305,0.000001920276,0.000009214046,0.00078101445,0.000059884514,0.0007824373],"genre_scores_gemma":[0.99725395,0.000087464476,0.0013369308,0.000036392354,0.0000067474057,0.000009631002,0.0010605283,0.000024832132,0.00018345276],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998965,0.000018605468,0.0000038874964,0.00002724489,0.000029705716,0.000024021047],"domain_scores_gemma":[0.9997851,0.000022016508,0.000066165805,0.000028925526,0.000025297837,0.0000725467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002718841,0.00017640101,0.00021575225,0.00077895145,0.00021421084,0.00038473247,0.00029794622,0.00025727806,0.00060436915],"category_scores_gemma":[0.0004603469,0.00015097686,0.00017670823,0.0006358733,0.00018935217,0.00020265626,0.00053534686,0.00018782984,0.00027114453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012298407,0.000098336975,0.94664603,0.000061439896,0.00011616989,0.00034085798,0.0009058355,0.0030542137,0.028829366,0.000300038,0.0019335597,0.017591218],"study_design_scores_gemma":[0.000010069702,0.000028649796,0.99582326,0.00001013422,0.000011897336,0.00007421354,0.00014061984,0.0025169817,0.0004952342,0.00006041389,0.00082416297,0.0000041916637],"about_ca_topic_score_codex":0.016221413,"about_ca_topic_score_gemma":0.033774935,"teacher_disagreement_score":0.016221413,"about_ca_system_score_codex":0.00029585554,"about_ca_system_score_gemma":0.0001951128,"threshold_uncertainty_score":0.03225398},"labels":[],"label_agreement":null},{"id":"W2996440992","doi":"10.3847/1538-4357/ab0d21","title":"The Green Bank North Celestial Cap Pulsar Survey. IV. Four New Timing Solutions","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"","keywords":"Pulsar; Millisecond pulsar; Binary pulsar; Pulsar planet; X-ray pulsar; Green Bank Telescope; Dispersion (optics); Compact star","score_opus":0.03489165111363082,"score_gpt":0.3041932989851686,"score_spread":0.26930164787153776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2996440992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.91570985,0.0031016236,0.01475561,0.0020361992,0.0006279521,0.0003269396,0.029660854,0.0010062365,0.03277474],"genre_scores_gemma":[0.91916484,0.001104958,0.038502097,0.0004168875,0.0003610893,0.000288791,0.033186957,0.00014976494,0.006824707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99947065,0.00008735779,0.000055582026,0.000114009505,0.00014034742,0.00013203961],"domain_scores_gemma":[0.99819225,0.00022924296,0.0005040742,0.00027835893,0.00050410395,0.0002920085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010664997,0.0007481445,0.00051248894,0.0051595056,0.0010463772,0.001931609,0.0008579032,0.0007937851,0.0037575124],"category_scores_gemma":[0.0026060543,0.00035031314,0.00039593206,0.00655092,0.00043058358,0.00048573423,0.000990262,0.00078974856,0.0012473173],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011558335,0.00014600567,0.7564742,0.00019358826,0.00017984849,0.0014755967,0.0006912013,0.008987182,0.0065069725,0.0035165441,0.026370669,0.19430229],"study_design_scores_gemma":[0.00039443388,0.00013441405,0.91179425,0.00012426786,0.00012721698,0.0006803394,0.000862381,0.020290222,0.0016657797,0.0016306562,0.062203035,0.00009296304],"about_ca_topic_score_codex":0.12277763,"about_ca_topic_score_gemma":0.25745374,"teacher_disagreement_score":0.12277763,"about_ca_system_score_codex":0.0024310353,"about_ca_system_score_gemma":0.0015392151,"threshold_uncertainty_score":0.24412596},"labels":[],"label_agreement":null},{"id":"W2996712626","doi":"10.3847/1538-4357/ab63df","title":"Detection of Missing Baryons in Galaxy Groups with Kinetic Sunyaev–Zel’dovich Effect","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Halo; Galaxy; Cosmic microwave background; Baryon; Galactic halo; Kinetic energy; Halo mass function; Galaxy formation and evolution; Sunyaev–Zel'dovich effect; Galaxy group","score_opus":0.00543899347894294,"score_gpt":0.19540035784969573,"score_spread":0.18996136437075278,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2996712626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987587,0.00010471052,0.00035931997,0.000012308093,0.000003253687,0.0000025287354,0.00012356356,0.000026101947,0.0006096413],"genre_scores_gemma":[0.99969316,0.000015471995,0.0001175796,0.0000031009308,0.0000029733242,0.000001005655,0.00012304692,0.0000026150858,0.00004113678],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997805,0.000028635988,0.000010184249,0.00005189018,0.000052363437,0.00007660466],"domain_scores_gemma":[0.9989215,0.00021047008,0.00037753838,0.00015582297,0.00006949754,0.0002652289],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033411323,0.00028049218,0.0003558899,0.00156269,0.00026525813,0.00062769273,0.00022939469,0.00018784076,0.0012376822],"category_scores_gemma":[0.00086151774,0.00020394746,0.00022838949,0.00057819753,0.00043916338,0.00023093943,0.0008030235,0.00017369578,0.00015925503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005019055,0.000033514305,0.94169164,0.000059146194,0.00015538027,0.00026996937,0.00026593858,0.00066720136,0.047630813,0.0005815607,0.00018270579,0.007960217],"study_design_scores_gemma":[0.000014404828,0.00004625817,0.9923044,0.000005987185,0.000041839266,0.00015385987,0.000084840336,0.0009113449,0.005738721,0.0002451329,0.00044545167,0.000007703301],"about_ca_topic_score_codex":0.00094675773,"about_ca_topic_score_gemma":0.0011928066,"teacher_disagreement_score":0.00156269,"about_ca_system_score_codex":0.00017433825,"about_ca_system_score_gemma":0.00009460866,"threshold_uncertainty_score":0.0041404963},"labels":[],"label_agreement":null},{"id":"W2997081985","doi":"10.3847/1538-4357/ab80bf","title":"Dynamical Simulations of the First Globular Clusters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Milky Way; Dark matter halo; Dark matter; Astronomy; Halo; Galaxy; Dwarf galaxy; Star cluster; Population; Velocity dispersion; Redshift; Stars","score_opus":0.01047112235265494,"score_gpt":0.2158920903563801,"score_spread":0.20542096800372517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2997081985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99207824,0.000071706825,0.0014838509,0.00018663514,0.000024218429,0.000033517917,0.00054954423,0.00013952833,0.005432587],"genre_scores_gemma":[0.9958949,0.0000396634,0.0018632177,0.00005732178,0.0000065186823,0.000045380646,0.00073856424,0.000043430475,0.0013110166],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998306,0.000040640934,0.000005997203,0.000030506833,0.00003304709,0.000059222344],"domain_scores_gemma":[0.99898916,0.0004059063,0.000064792235,0.00008511915,0.00018480628,0.0002701322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048304012,0.0003860042,0.0005220243,0.0006162631,0.0009670085,0.00090567005,0.0014507283,0.0009991075,0.0032961126],"category_scores_gemma":[0.0024353398,0.00041056293,0.00076006196,0.00061261444,0.00092906214,0.00054237986,0.0010251128,0.00089323666,0.0002752975],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002492701,0.00015665981,0.017286338,0.00003954922,0.00009913039,0.00020906399,0.00020126723,0.9734423,0.0014371348,0.0034072418,0.0012553802,0.0022167275],"study_design_scores_gemma":[0.00014443912,0.00008993619,0.0049987338,0.000011824894,0.00002499394,0.000026324773,0.00010175489,0.99161255,0.0007694129,0.00086170074,0.001340785,0.000017513434],"about_ca_topic_score_codex":0.051597066,"about_ca_topic_score_gemma":0.032389075,"teacher_disagreement_score":0.051597066,"about_ca_system_score_codex":0.0020660118,"about_ca_system_score_gemma":0.0013925511,"threshold_uncertainty_score":0.10259348},"labels":[],"label_agreement":null},{"id":"W2997522131","doi":"10.3847/1538-4357/ab58d2","title":"Hubble Space Telescope Imaging of Antlia B: Star Formation History and a New Tip of the Red Giant Branch Distance","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Physics; Hubble space telescope; Astronomy; Astrophysics; Red-giant branch; Star formation; Star (game theory); Stars; Globular cluster","score_opus":0.012733849562487838,"score_gpt":0.19915438751635414,"score_spread":0.18642053795386632,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2997522131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960582,0.000095489064,0.00025735205,0.000042815744,0.000003884262,0.0000045838246,0.0006244533,0.000044971443,0.0028683024],"genre_scores_gemma":[0.99783796,0.00003130621,0.0008287357,0.000021302974,0.000004785215,0.0000020802197,0.00068357267,0.000007962906,0.0005822143],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999399,0.000003142439,0.0000027368565,0.000018602106,0.000020699492,0.000014815623],"domain_scores_gemma":[0.9996791,0.000017243006,0.00009239525,0.000021613923,0.000047955786,0.00014177062],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009215738,0.00011794619,0.000105144536,0.0009014141,0.00025430863,0.00037755244,0.00018730886,0.00023959157,0.0014828927],"category_scores_gemma":[0.00021384942,0.000105104744,0.00009461371,0.00034002875,0.00013125488,0.00019275976,0.0002878288,0.00021979949,0.0005286321],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020319477,0.000043481683,0.8931109,0.000025946028,0.00002403518,0.0005096368,0.00025015682,0.00024416926,0.09327262,0.00016874913,0.0013695722,0.0107775135],"study_design_scores_gemma":[0.0000011033968,0.000009262095,0.9984718,0.0000020049183,0.0000015685813,0.00021946222,0.000033047025,0.00018643252,0.00058656797,0.000019523439,0.00046792004,0.0000013188891],"about_ca_topic_score_codex":0.009156977,"about_ca_topic_score_gemma":0.021868555,"teacher_disagreement_score":0.009156977,"about_ca_system_score_codex":0.0003138653,"about_ca_system_score_gemma":0.00009660665,"threshold_uncertainty_score":0.018207371},"labels":[],"label_agreement":null},{"id":"W2997604591","doi":"10.3847/1538-4357/ab7b67","title":"Modeling the Uncertainties of Solar System Ephemerides for Robust Gravitational-wave Searches with Pulsar-timing Arrays","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"Office of Naval Research; Science and Technology Facilities Council; Flatiron Health; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Aspen Center for Physics; University of Wisconsin-Milwaukee; National Aeronautics and Space Administration; California Institute of Technology; Oak Ridge Associated Universities; University of Central Florida; National Science Foundation","keywords":"Ephemeris; Pulsar; Physics; Binary pulsar; Solar System; Gravitational wave; Astronomy; Astrophysics; Gravitational-wave observatory; Millisecond pulsar; Satellite","score_opus":0.0626402240883001,"score_gpt":0.30123202681066796,"score_spread":0.23859180272236785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2997604591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6993546,0.00017638197,0.29618812,0.000392774,0.000021641861,0.000040568895,0.0004516345,0.00022696739,0.003147247],"genre_scores_gemma":[0.98981655,0.00004717097,0.009646032,0.000020432833,0.000007743597,0.000023906909,0.00012880271,0.000023926888,0.00028545788],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99960035,0.0001844892,0.000021639486,0.00007262314,0.00007772757,0.000043205917],"domain_scores_gemma":[0.99532485,0.003763685,0.00048529648,0.00020325197,0.00015130122,0.000071665934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021300511,0.0003223326,0.0004563679,0.00037552952,0.000316303,0.00091501453,0.0007214218,0.0005193484,0.0005321491],"category_scores_gemma":[0.009060104,0.00028218792,0.00039889183,0.00048218254,0.00059307046,0.0010377824,0.0006605806,0.0006908811,0.00007460715],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022824759,0.000008225514,0.0023308059,0.0000056576278,0.000010938935,0.000011927557,0.000012363206,0.9920433,0.00024966497,0.0041321474,0.000055399014,0.001116805],"study_design_scores_gemma":[0.0000021717492,0.000005996975,0.00046208594,0.0000015275268,0.000002280432,0.0000026082198,0.0000037458885,0.9981463,0.00014780356,0.0011725187,0.000050727736,0.000002252055],"about_ca_topic_score_codex":0.009747774,"about_ca_topic_score_gemma":0.0055870684,"teacher_disagreement_score":0.009747774,"about_ca_system_score_codex":0.0009470125,"about_ca_system_score_gemma":0.00065125176,"threshold_uncertainty_score":0.01938206},"labels":[],"label_agreement":null},{"id":"W2997939585","doi":"10.3847/1538-4357/ab67bc","title":"Absolute Calibration Strategies for the Hydrogen Epoch of Reionization Array and Their Impact on the 21 cm Power Spectrum","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Reionization; HERA; Calibration; Epoch (astronomy); Estimator; Sky; Spectral density; Phase (matter)","score_opus":0.013227245530230212,"score_gpt":0.22530967555867995,"score_spread":0.21208243002844973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2997939585","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26202923,0.00055282796,0.7279339,0.00057368743,0.00008755931,0.00005743539,0.00025041858,0.0015952109,0.0069197076],"genre_scores_gemma":[0.7425814,0.00014864838,0.25526807,0.00010087669,0.000032000342,0.00004571962,0.00032996593,0.00029925228,0.0011940823],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9991498,0.00024542524,0.000033426044,0.00019693279,0.00030322684,0.0000710777],"domain_scores_gemma":[0.99815077,0.00052735076,0.00033179732,0.00052465824,0.0003881759,0.000077335266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023352471,0.0005627611,0.00025465438,0.0009505013,0.00042605412,0.0009321638,0.00091332354,0.000520211,0.0014139754],"category_scores_gemma":[0.0069321063,0.00029888054,0.00036901014,0.0006796903,0.00040548312,0.0010573933,0.0012681325,0.0007839877,0.0005309663],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005592267,0.00015668286,0.049806654,0.00018537368,0.00022718686,0.0001170851,0.0006407541,0.28374633,0.104296885,0.050240543,0.00362567,0.50639755],"study_design_scores_gemma":[0.0000637976,0.00022292216,0.040922638,0.00009394405,0.00009226989,0.0002778307,0.00023303389,0.8484752,0.07620664,0.021930428,0.01137095,0.00011034396],"about_ca_topic_score_codex":0.001964854,"about_ca_topic_score_gemma":0.0027949812,"teacher_disagreement_score":0.0023352471,"about_ca_system_score_codex":0.000638546,"about_ca_system_score_gemma":0.00062236964,"threshold_uncertainty_score":0.012350142},"labels":[],"label_agreement":null},{"id":"W2997940382","doi":"10.3847/1538-4357/ab855e","title":"The Gravitational Wave Treasure Map: A Tool to Coordinate, Visualize, and Assess the Electromagnetic Follow-up of Gravitational-wave Events","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; University of Toronto","funders":"","keywords":"Treasure; Gravitational wave; Gravitation; Electromagnetic radiation; Square (algebra); Electromagnetic spectrum","score_opus":0.023878508725177727,"score_gpt":0.31478693266603475,"score_spread":0.29090842394085703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2997940382","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.02425615,0.0009354609,0.37431198,0.0012481981,0.00047783565,0.0004494743,0.047864888,0.52531165,0.025144296],"genre_scores_gemma":[0.26634827,0.0014976285,0.5661219,0.0009177945,0.00049856387,0.0014464238,0.06434993,0.07897008,0.019849543],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9994636,0.00010889842,0.000044638535,0.000100338475,0.00021136052,0.00007111779],"domain_scores_gemma":[0.9965179,0.0015111386,0.00038373243,0.0005493647,0.0004432891,0.00059455354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011851151,0.0013614324,0.0009306685,0.00521314,0.0008915735,0.0031949044,0.0017106362,0.0011659702,0.03547509],"category_scores_gemma":[0.007903275,0.0006459973,0.0009535422,0.0028516122,0.0005563614,0.0034186856,0.0051989257,0.0014242323,0.012688625],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011865447,0.00025286013,0.016365793,0.0011201479,0.00034739915,0.0014570188,0.0021988791,0.007838573,0.0097662555,0.016776247,0.6339266,0.3087637],"study_design_scores_gemma":[0.00066718983,0.00024131058,0.02729892,0.0005614643,0.00021435363,0.0015712888,0.00109463,0.14085223,0.02768166,0.05961666,0.73957586,0.0006244165],"about_ca_topic_score_codex":0.0032263708,"about_ca_topic_score_gemma":0.003885366,"teacher_disagreement_score":0.03547509,"about_ca_system_score_codex":0.00038251956,"about_ca_system_score_gemma":0.0009010655,"threshold_uncertainty_score":0.11867607},"labels":[],"label_agreement":null},{"id":"W2998036038","doi":"10.3847/1538-4357/ab6602","title":"A Convective Dredge-up Model as the Origin of Hydrogen in DBA White Dwarfs","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"White dwarf; Convection; Hydrogen; Radiative transfer; Convection zone; Context (archaeology); Accretion (finance); Helium; Blue dwarf","score_opus":0.018166753987538684,"score_gpt":0.25279888554204377,"score_spread":0.23463213155450507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2998036038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94979054,0.00022575477,0.039919674,0.00025248638,0.0000328577,0.000031617874,0.00016111488,0.00010337049,0.009482595],"genre_scores_gemma":[0.99455845,0.00009872365,0.0032439926,0.000032070686,0.000012532512,0.00002181286,0.00004579907,0.00002104746,0.001965476],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999485,0.000014708923,0.0000031689463,0.000010233652,0.000011623805,0.000011611971],"domain_scores_gemma":[0.9998574,0.00003768935,0.000019655505,0.000023172217,0.00002096906,0.000041101226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023678556,0.00026936125,0.00051533815,0.00025454658,0.0005758708,0.0007370647,0.0010230361,0.0005685597,0.00092453347],"category_scores_gemma":[0.00042172623,0.00021589549,0.0005581008,0.00016810783,0.00043940565,0.0006804373,0.0007021523,0.00033941146,0.00016893506],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009067902,0.00008383016,0.009121843,0.00003593201,0.00004526582,0.00040991744,0.00023125332,0.9433859,0.011984983,0.03192363,0.00026222735,0.0024245717],"study_design_scores_gemma":[0.00002806599,0.00002200439,0.0009797885,0.0000025409067,0.000011421149,0.00003309455,0.000027966333,0.99508864,0.00076525146,0.0025057553,0.0005298425,0.000005630236],"about_ca_topic_score_codex":0.013916729,"about_ca_topic_score_gemma":0.0052812262,"teacher_disagreement_score":0.013916729,"about_ca_system_score_codex":0.00078983855,"about_ca_system_score_gemma":0.00053207,"threshold_uncertainty_score":0.027671456},"labels":[],"label_agreement":null},{"id":"W2998201360","doi":"10.3847/1538-4357/ab4999","title":"A New Sample of (Wandering) Massive Black Holes in Dwarf Galaxies from High-resolution Radio Observations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":217,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Ministério da Ciência, Tecnologia e Inovação; Chinese Academy of Sciences; High Energy Physics; Deutsche Forschungsgemeinschaft; University of Sussex; University of Oxford; York University; National Energy Research Scientific Computing Center; Leibniz-Gemeinschaft; University of Notre Dame; National Aeronautics and Space Administration; University College London; Carnegie Mellon University; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Vanderbilt University; University of Chicago; Ohio State University; Fermilab; National Science Foundation; New Mexico State University; University of Portsmouth; Yale University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; Financiadora de Estudos e Projetos; University of Pennsylvania","keywords":"Dwarf galaxy; Jansky; Galaxy; Radio galaxy; Population; Dwarf spheroidal galaxy; Elliptical galaxy; Peculiar galaxy; Dwarf galaxy problem","score_opus":0.0195024152498652,"score_gpt":0.2120525453903324,"score_spread":0.19255013014046718,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2998201360","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951625,0.00004447329,0.00015838978,0.0000058475343,0.0000013105728,0.000006815603,0.00014185706,0.0000052905966,0.00011971829],"genre_scores_gemma":[0.99857867,0.00004191919,0.0003716485,0.000016894426,0.000008076249,0.0000048762877,0.00074020465,0.0000035563178,0.00023417559],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997862,0.000026812046,0.000018305374,0.00006540756,0.000055797387,0.00004745689],"domain_scores_gemma":[0.9995413,0.00006593289,0.00011205223,0.000081189915,0.000047537298,0.00015206308],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003115171,0.00023708827,0.00026183957,0.0011722049,0.00031239804,0.00064042193,0.0002588972,0.00016429964,0.0008673878],"category_scores_gemma":[0.000647801,0.0001767411,0.00020751398,0.0005000986,0.00024177277,0.00030079868,0.0005998022,0.00017337478,0.00029372575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008726671,0.00005691261,0.9841293,0.00001173925,0.000027768538,0.00025872525,0.00029124625,0.000051067487,0.009674069,0.00004105697,0.00012442515,0.0052463114],"study_design_scores_gemma":[0.000004894334,0.00004166096,0.99817634,0.0000015646335,0.000014173939,0.00047330983,0.00013986269,0.00013992553,0.00057805766,0.000015898011,0.00041224156,0.0000021935332],"about_ca_topic_score_codex":0.0016461327,"about_ca_topic_score_gemma":0.0033400676,"teacher_disagreement_score":0.0016461327,"about_ca_system_score_codex":0.00009661937,"about_ca_system_score_gemma":0.00009477227,"threshold_uncertainty_score":0.0032731295},"labels":[],"label_agreement":null},{"id":"W2998821518","doi":"10.3847/1538-4357/ab6b2a","title":"Thirty Years of Radio Observations of Type Ia SN 1972E and SN 1895B: Constraints on Circumstellar Shells","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"White dwarf; Supernova; Pair-instability supernova; Stars; Envelope (radar); Degenerate energy levels; Stellar evolution","score_opus":0.025518537040461253,"score_gpt":0.23798603668440702,"score_spread":0.21246749964394576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2998821518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977163,0.00028591632,0.0001593057,0.000019593168,0.000005733279,0.0000035888074,0.0006640805,0.000010081958,0.0011353416],"genre_scores_gemma":[0.9970176,0.00013678627,0.00016231228,0.000021342108,0.00001151629,0.0000036512429,0.0022718266,0.0000034468471,0.0003714834],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.000010001371,0.000009562761,0.000024772098,0.000039096612,0.00003435954],"domain_scores_gemma":[0.9995517,0.00006477587,0.00013725772,0.00003638709,0.00008166992,0.00012823533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028501588,0.0001359492,0.00018526956,0.0008899982,0.00028090805,0.0005542416,0.00013414511,0.00019784832,0.0007469808],"category_scores_gemma":[0.00046483736,0.00010392,0.00014309071,0.0004324235,0.0001794987,0.00021307761,0.00037611046,0.00014411192,0.00029697805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027246115,0.00006857375,0.9676908,0.000042169773,0.00009142499,0.0007134633,0.00020561328,0.00047006382,0.019155735,0.00012040968,0.0005665911,0.010602769],"study_design_scores_gemma":[0.0000027478545,0.000019902413,0.9969998,0.000004872535,0.000011092753,0.00018712971,0.00006880698,0.00015129936,0.0008302663,0.000013144885,0.0017064797,0.0000043959694],"about_ca_topic_score_codex":0.0073420545,"about_ca_topic_score_gemma":0.018211666,"teacher_disagreement_score":0.0073420545,"about_ca_system_score_codex":0.0002536178,"about_ca_system_score_gemma":0.00012499258,"threshold_uncertainty_score":0.014598608},"labels":[],"label_agreement":null},{"id":"W2999217829","doi":"10.3847/1538-4357/ab6992","title":"The PIPER Survey. I. An Initial Look at the Intergalactic Globular Cluster Population in the Perseus Cluster","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics; McMaster University","funders":"","keywords":"Physics; Astrophysics; Globular cluster; Intergalactic travel; Astronomy; Galaxy cluster; Brightest cluster galaxy; Elliptical galaxy; Galaxy; Intracluster medium; Redshift","score_opus":0.015469315726353655,"score_gpt":0.24729440723930782,"score_spread":0.23182509151295416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999217829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9838949,0.0002214289,0.00054554624,0.00020721705,0.000006036133,0.000066504224,0.009329032,0.00009702283,0.005632397],"genre_scores_gemma":[0.9783271,0.00023114996,0.002321708,0.00016140038,0.000021437176,0.000064028456,0.015145509,0.000021930122,0.0037056617],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998975,0.000020623464,0.0000046778036,0.00003691736,0.000020657633,0.000019716561],"domain_scores_gemma":[0.9997632,0.0000177793,0.000054442393,0.00003789967,0.000048315003,0.00007836154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002729227,0.00029628177,0.00012218262,0.0007951228,0.00020488242,0.00020946826,0.00028311953,0.00014041114,0.003179709],"category_scores_gemma":[0.000329488,0.00011523999,0.00007762933,0.0005579857,0.00015484839,0.0004273588,0.00068792095,0.00015276964,0.00081637775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007053429,0.00010239768,0.9092652,0.000090451074,0.00004584664,0.00057823444,0.00089855905,0.0005456735,0.014611248,0.0006090061,0.008416199,0.064131826],"study_design_scores_gemma":[0.000020503558,0.00006388213,0.9934576,0.0000063176512,0.0000068765416,0.00019409721,0.00025955573,0.00025193713,0.0007015718,0.00008317962,0.004951294,0.0000032023322],"about_ca_topic_score_codex":0.010709368,"about_ca_topic_score_gemma":0.020767312,"teacher_disagreement_score":0.010709368,"about_ca_system_score_codex":0.00029831147,"about_ca_system_score_gemma":0.00016973463,"threshold_uncertainty_score":0.021294057},"labels":[],"label_agreement":null},{"id":"W2999294010","doi":"10.3847/1538-4357/ab6f72","title":"Discovery of a Remarkably Powerful Broad Absorption-line Quasar Outflow in SDSS J135246.37+423923.5","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; Western University","funders":"","keywords":"Quasar; Outflow; Astrophysics; Astronomy; Line (geometry); Second line; Absorption spectroscopy; Physics; Optics; First line; Medicine; Galaxy; Mathematics; Meteorology","score_opus":0.017050542408974544,"score_gpt":0.24235341388367954,"score_spread":0.22530287147470499,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999294010","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99920183,0.000022591164,0.00023532947,0.000013185405,0.000002479015,0.0000034447821,0.0001485163,0.00003630608,0.00033625655],"genre_scores_gemma":[0.99924904,0.000007911583,0.0003645981,0.000013197376,0.0000024752785,0.0000018212213,0.00025468937,0.0000069535267,0.00009923864],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992704,0.0000044325784,0.0000032958665,0.000024032872,0.000021328262,0.000019820778],"domain_scores_gemma":[0.9998386,0.0000111490845,0.000046974015,0.000011870142,0.000013227421,0.0000781809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015545126,0.00025361925,0.00023904555,0.0007014143,0.0004103874,0.0005336229,0.00029225225,0.00020406203,0.0007815671],"category_scores_gemma":[0.00018870602,0.00014392791,0.00019486478,0.00031002975,0.00025726485,0.00012569717,0.0004972102,0.00019948551,0.00013391991],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003304649,0.00016796691,0.48726806,0.00007417517,0.00013158518,0.004430414,0.000698357,0.0012693483,0.48588532,0.0012261393,0.000950242,0.01756788],"study_design_scores_gemma":[0.00002601887,0.00008423307,0.9832146,0.000005381452,0.000033636385,0.00082093553,0.00019769296,0.0036551042,0.009779005,0.00021475807,0.0019527157,0.000015883325],"about_ca_topic_score_codex":0.0038294354,"about_ca_topic_score_gemma":0.006752875,"teacher_disagreement_score":0.0038294354,"about_ca_system_score_codex":0.00035832424,"about_ca_system_score_gemma":0.00013645727,"threshold_uncertainty_score":0.0076143146},"labels":[],"label_agreement":null},{"id":"W2999297823","doi":"10.3847/1538-4357/ab59d0","title":"Gravity-darkening Analysis of the Misaligned Hot Jupiter MASCARA-4 b","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science Mission Directorate; Goddard Space Flight Center; Universities Space Research Association; Ames Research Center; National Aeronautics and Space Administration","keywords":"Exoplanet; Planet; Eclipse; Hot Jupiter; Orbit (dynamics); Transit (satellite); Jupiter (rocket family); Orbital decay; Orbital inclination; Orbital eccentricity","score_opus":0.012370277958129445,"score_gpt":0.22465279664975404,"score_spread":0.2122825186916246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999297823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99810565,0.00003637959,0.0006448658,0.000015953901,0.0000036884305,0.0000053772287,0.00021953305,0.00006194505,0.000906514],"genre_scores_gemma":[0.9986834,0.00001308887,0.00060741423,0.000009227835,0.0000026782047,0.0000028917455,0.0004454611,0.000017725715,0.00021809377],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999113,0.00001199895,0.0000031858763,0.000036389905,0.00001909285,0.00001798964],"domain_scores_gemma":[0.99972755,0.000029021674,0.00007619514,0.0000474714,0.00004514598,0.000074600284],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002115172,0.000334793,0.00023632658,0.0007397097,0.0005108358,0.00036984606,0.00046361116,0.00034530967,0.0011107615],"category_scores_gemma":[0.00034497303,0.00019899274,0.00043375036,0.00043117587,0.00025143957,0.00021150347,0.0004547624,0.00020212769,0.00034686053],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063543516,0.00018011224,0.8258261,0.000066081004,0.00019054148,0.0005512239,0.00032441746,0.036761824,0.120793626,0.0012824158,0.0016498691,0.011738423],"study_design_scores_gemma":[0.000023860377,0.0002465941,0.88877755,0.000007522047,0.00003952299,0.0002457389,0.00012772325,0.10160992,0.006570885,0.0003038533,0.0020197462,0.000027078868],"about_ca_topic_score_codex":0.018370768,"about_ca_topic_score_gemma":0.014974119,"teacher_disagreement_score":0.018370768,"about_ca_system_score_codex":0.0006209532,"about_ca_system_score_gemma":0.00016148727,"threshold_uncertainty_score":0.036527693},"labels":[],"label_agreement":null},{"id":"W2999554518","doi":"10.3847/1538-4357/ab6082","title":"Constraints on Cosmological Parameters from the 500 deg<sup>2</sup> SPTPOL Lensing Power Spectrum","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":87,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"Argonne National Laboratory; National Energy Research Scientific Computing Center; Science and Technology Facilities Council; Office of Science; University of Chicago; U.S. Department of Energy","keywords":"Physics; Cosmic microwave background; Planck; Omega; Spectral density; Astrophysics; Baryon; Lambda; Weak gravitational lensing; Sigma; Particle physics; Dark energy; Cosmology; Redshift; Astronomy; Quantum mechanics; Anisotropy; Galaxy; Statistics","score_opus":0.017356851625723264,"score_gpt":0.23708997237988988,"score_spread":0.21973312075416662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999554518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9681551,0.00032283834,0.011064345,0.0003777105,0.000022502945,0.000011644208,0.005313902,0.0004404256,0.014291491],"genre_scores_gemma":[0.99404955,0.0001178691,0.0017817473,0.000051155417,0.000020488225,0.000008606584,0.0035558392,0.00008589442,0.0003288427],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99964774,0.00010113548,0.000017122416,0.00006867896,0.000103333696,0.00006198908],"domain_scores_gemma":[0.99789137,0.0009768043,0.0004041317,0.00034253296,0.00024063734,0.00014457798],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007552383,0.0010158293,0.00037833015,0.0011871125,0.00031857943,0.0017245552,0.0005449485,0.0004907996,0.006877173],"category_scores_gemma":[0.004029262,0.0004145255,0.0007882448,0.0012863575,0.00042885574,0.00073352986,0.0006657293,0.00046159903,0.0014935092],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009804413,0.000097214135,0.64052916,0.0003600137,0.0010317966,0.001308931,0.0004057939,0.21864837,0.040868808,0.02386441,0.011402799,0.060502343],"study_design_scores_gemma":[0.000058451034,0.00007638049,0.7534939,0.00012191155,0.00031678498,0.00032854307,0.00035537104,0.19816098,0.019056046,0.012688444,0.0152148865,0.00012826787],"about_ca_topic_score_codex":0.010771492,"about_ca_topic_score_gemma":0.011643207,"teacher_disagreement_score":0.010771492,"about_ca_system_score_codex":0.00073880976,"about_ca_system_score_gemma":0.00030707457,"threshold_uncertainty_score":0.023006499},"labels":[],"label_agreement":null},{"id":"W2999610399","doi":"10.3847/1538-4357/ab68dc","title":"The Large-scale Behavior in the Disk of δ Scorpii from 2000 to 2018","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Plant-based Medicinal Research","field":"Pharmacology, Toxicology and Pharmaceutics","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Scale (ratio); Physics","score_opus":0.10775008853487479,"score_gpt":0.4336518552431951,"score_spread":0.32590176670832033,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999610399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99671715,0.0001004839,0.00065279426,0.00013813045,0.000007278807,0.0000071854356,0.00045161342,0.00007164133,0.0018537272],"genre_scores_gemma":[0.9991033,0.000048695696,0.0001910904,0.00001861425,0.0000036517242,0.0000056645863,0.0002996059,0.000013282999,0.00031608285],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.000008747893,0.0000028656207,0.000022064069,0.000010407687,0.000018501883],"domain_scores_gemma":[0.99969244,0.00009010045,0.000074079995,0.00003282784,0.00005310439,0.00005735179],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022581172,0.00033430662,0.00020756858,0.00048041443,0.00058885984,0.00078649406,0.00063237007,0.00071171485,0.0015194193],"category_scores_gemma":[0.0013282836,0.00025687,0.0003906329,0.00045595068,0.00050448405,0.00060585944,0.0003546618,0.00039649187,0.00026684982],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000268874,0.00013555518,0.3340519,0.000077509074,0.00012454603,0.0007647563,0.00030664323,0.64448404,0.00936359,0.002266717,0.0012744954,0.0068813725],"study_design_scores_gemma":[0.00008251404,0.00010412136,0.24297073,0.000036533864,0.00007362891,0.00031702314,0.00028879588,0.74899185,0.0030856777,0.0014389852,0.0025566167,0.000053517913],"about_ca_topic_score_codex":0.045062434,"about_ca_topic_score_gemma":0.018504385,"teacher_disagreement_score":0.045062434,"about_ca_system_score_codex":0.0015566472,"about_ca_system_score_gemma":0.000436696,"threshold_uncertainty_score":0.089600265},"labels":[],"label_agreement":null},{"id":"W2999736717","doi":"10.3847/1538-4357/ab7b66","title":"Gravitational-wave Detection and Parameter Estimation for Accreting Black-hole Binaries and Their Electromagnetic Counterpart","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Generalitat Valenciana","keywords":"Accretion (finance); Interferometry; Redshift; Sky; Parameter space; Accretion disc; Observable","score_opus":0.015814297790945835,"score_gpt":0.28309463465947815,"score_spread":0.2672803368685323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W2999736717","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99693847,0.000052663923,0.0026087058,0.000015682044,0.0000027155186,0.000004550275,0.00010580752,0.000043120297,0.00022829982],"genre_scores_gemma":[0.99716693,0.000016675964,0.002427702,0.0000039562906,0.0000055338296,0.0000029502446,0.0002869736,0.000006787358,0.00008246881],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998629,0.000040823033,0.000009405475,0.00003057522,0.000030782714,0.0000255543],"domain_scores_gemma":[0.99918574,0.00036681938,0.00019416084,0.000062104176,0.00008230213,0.000108827764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059793144,0.00026206835,0.00028331557,0.0014030734,0.00019626928,0.0004983311,0.00027718057,0.00030522115,0.0006100354],"category_scores_gemma":[0.00210558,0.00014366876,0.00020394358,0.0005313156,0.0001350538,0.00037459808,0.0004543304,0.00021212873,0.00020466687],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000867872,0.00019602751,0.8943157,0.000043908454,0.00013523725,0.00024581637,0.000086764965,0.03218442,0.029910496,0.0007137225,0.00026713643,0.041032843],"study_design_scores_gemma":[0.000036270914,0.00015150243,0.59241414,0.000007776207,0.000033552857,0.00019077728,0.00008853331,0.3955198,0.010707909,0.0005295487,0.00029874325,0.000021450536],"about_ca_topic_score_codex":0.002854123,"about_ca_topic_score_gemma":0.002578101,"teacher_disagreement_score":0.002854123,"about_ca_system_score_codex":0.00026646568,"about_ca_system_score_gemma":0.00020067039,"threshold_uncertainty_score":0.005675018},"labels":[],"label_agreement":null},{"id":"W3000030301","doi":"10.3847/1538-4357/ab659e","title":"Detection of Irregular, Submillimeter Opaque Structures in the Orion Molecular Clouds: Protostars within 10,000 yr of Formation?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"National Aeronautics and Space Administration","keywords":"Protostar; Opacity; Submillimeter Array; Substructure; Outflow; Molecular cloud; Hydrostatic equilibrium; Orion Nebula; Millimeter","score_opus":0.010494466127162327,"score_gpt":0.22844875684978394,"score_spread":0.21795429072262162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3000030301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994758,0.000088013585,0.0001091345,0.000020640968,0.000003034849,0.0000017731719,0.000046463178,0.000008105397,0.00024716082],"genre_scores_gemma":[0.9993531,0.000046382924,0.00023746368,0.000016657614,0.0000075094417,0.0000022471656,0.00018009482,0.0000024698086,0.00015400934],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999033,0.000008453591,0.000005571057,0.000028218332,0.000020571608,0.00003379164],"domain_scores_gemma":[0.999485,0.00006569312,0.00021168965,0.00004633864,0.000046299327,0.00014490336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028867138,0.00014030194,0.00017999968,0.00043426565,0.00033454032,0.0005715055,0.00029862532,0.00042077975,0.0009468758],"category_scores_gemma":[0.0005680938,0.00015396501,0.00013382953,0.0002995298,0.00028976,0.0003599116,0.00037564966,0.00028902554,0.00028457548],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010901151,0.000041578034,0.9632545,0.000017923227,0.000023149694,0.00043014804,0.00031674415,0.00014002695,0.03067152,0.0001368332,0.00012916776,0.0047294586],"study_design_scores_gemma":[0.0000024614292,0.000042373875,0.99770796,0.000004292743,0.0000067015417,0.0002816222,0.000120425626,0.00027265007,0.00092120684,0.0000615267,0.00057610526,0.0000026743187],"about_ca_topic_score_codex":0.001345813,"about_ca_topic_score_gemma":0.0034078278,"teacher_disagreement_score":0.001345813,"about_ca_system_score_codex":0.00034354374,"about_ca_system_score_gemma":0.00010838401,"threshold_uncertainty_score":0.0031676292},"labels":[],"label_agreement":null},{"id":"W3000087935","doi":"10.3847/1538-4357/ab660c","title":"Two New Outbursts and Transient Hard X-Rays from 1E 1048.1-5937","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Amplitude; Black-body radiation; Light curve; Transient (computer programming); Radiative transfer; Telescope; Erg; Observatory","score_opus":0.02330002787862528,"score_gpt":0.23217645520924624,"score_spread":0.20887642733062095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3000087935","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985695,0.00011103921,0.00020419517,0.000030039384,0.000018515553,0.000012438404,0.00020308315,0.000029598328,0.00082162203],"genre_scores_gemma":[0.99755543,0.00007075716,0.00048139377,0.000055574754,0.00003134274,0.000014713013,0.0011656532,0.000016661093,0.0006085518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998223,0.0000098413675,0.000011294359,0.000054380645,0.000042892294,0.000059244674],"domain_scores_gemma":[0.99938536,0.00006870592,0.00018393359,0.00007547584,0.000071417315,0.0002151095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002583971,0.00032693098,0.00043034783,0.000719879,0.00060051034,0.00043952503,0.00028140153,0.00032388052,0.0009777327],"category_scores_gemma":[0.00045234323,0.00018693079,0.00025688027,0.00036008935,0.0002541305,0.00023087757,0.00065923657,0.0006044158,0.0002763839],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00064559485,0.00044292322,0.8392116,0.000100114165,0.00010237635,0.005482211,0.0016533425,0.00032526063,0.12530778,0.00028111227,0.0019964084,0.024451124],"study_design_scores_gemma":[0.0000104528335,0.00013118214,0.9947003,0.0000105514455,0.000016023712,0.0010404012,0.00018745313,0.00020806874,0.0019558016,0.000048722206,0.0016837672,0.0000072564],"about_ca_topic_score_codex":0.0021018663,"about_ca_topic_score_gemma":0.0065660253,"teacher_disagreement_score":0.0021018663,"about_ca_system_score_codex":0.0002851512,"about_ca_system_score_gemma":0.00010406378,"threshold_uncertainty_score":0.0041791797},"labels":[],"label_agreement":null},{"id":"W3000714584","doi":"10.3847/1538-4357/ab66b1","title":"The Effects of Plasma Lensing on the Inferred Dispersion Measures of Fast Radiobursts","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"National Natural Science Foundation of China","keywords":"Plasma; Dispersion (optics); Gravitational lens; Line (geometry); Plasma oscillation; Electron; Electron density; Optical depth","score_opus":0.01565209232002201,"score_gpt":0.21044538429145146,"score_spread":0.19479329197142944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3000714584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9856844,0.0005794378,0.012352319,0.000060448318,0.000014195971,0.000005601958,0.00035146845,0.0001287378,0.0008233689],"genre_scores_gemma":[0.9981737,0.00005497874,0.0014952404,0.000007982476,0.000010565998,0.0000020978466,0.00019677157,0.000016734148,0.000041928295],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992055,0.00030393546,0.00006006423,0.0001905856,0.00016300887,0.000076827055],"domain_scores_gemma":[0.9862183,0.009810035,0.0022090091,0.000867404,0.0006486839,0.00024655604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002586681,0.00035007478,0.00020977246,0.0012587395,0.00023846507,0.00087411655,0.00044343693,0.00037350066,0.00045657132],"category_scores_gemma":[0.015323576,0.00023916225,0.0002542657,0.0007698437,0.0004227321,0.0006810426,0.0005496693,0.00029764473,0.000105847015],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009523784,0.00003620934,0.85758996,0.00022860273,0.00055731117,0.0005128999,0.0003602431,0.069882356,0.029710554,0.0029618554,0.0004904469,0.03671724],"study_design_scores_gemma":[0.000035058685,0.000101444115,0.7970191,0.000050503917,0.00017735873,0.0007120608,0.00014080522,0.17439745,0.023881001,0.0020538655,0.0013538337,0.00007748724],"about_ca_topic_score_codex":0.0029445442,"about_ca_topic_score_gemma":0.0020732651,"teacher_disagreement_score":0.0029445442,"about_ca_system_score_codex":0.00057166594,"about_ca_system_score_gemma":0.00014372027,"threshold_uncertainty_score":0.013679802},"labels":[],"label_agreement":null},{"id":"W3001681068","doi":"10.3847/1538-4357/ab7000","title":"A Model for the Onset of Self-gravitation and Star Formation in Molecular Gas Governed by Galactic Forces. II. The Bottleneck to Collapse Set by Cloud–Environment Decoupling","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Star formation; Galaxy; Molecular cloud; Milky Way; Gravitational collapse; Protogalaxy; Galaxy formation and evolution; Stars; Virial theorem","score_opus":0.01082471965377435,"score_gpt":0.22889613743106305,"score_spread":0.2180714177772887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3001681068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94947654,0.0009979693,0.037479665,0.0021828283,0.000060259452,0.00007516393,0.0002580403,0.00017524604,0.009294332],"genre_scores_gemma":[0.9946272,0.00024846962,0.0015382182,0.00009881129,0.00003148545,0.000045629065,0.000048770922,0.000024232673,0.003337081],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984777,0.000027271351,0.0000067810774,0.00003860568,0.000020731643,0.000058741247],"domain_scores_gemma":[0.99956113,0.00008806418,0.000108559376,0.00003098752,0.000046348752,0.0001649274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046920255,0.00059993315,0.0007875004,0.0006668027,0.0006404418,0.001239332,0.0016865362,0.0016352923,0.0026748613],"category_scores_gemma":[0.0009527112,0.0005684011,0.0009630265,0.00031784133,0.0013211985,0.0025878106,0.001474869,0.0009553923,0.00062317715],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004893476,0.00032385153,0.038503394,0.00022134265,0.00014843083,0.0014753727,0.00077531,0.63742834,0.042943045,0.2657752,0.0027401254,0.009176236],"study_design_scores_gemma":[0.00010269319,0.00014134406,0.009779863,0.000017068585,0.000031377112,0.0002298487,0.00010734498,0.95202583,0.0010771091,0.03501003,0.0014429529,0.000034544064],"about_ca_topic_score_codex":0.009793244,"about_ca_topic_score_gemma":0.0036921373,"teacher_disagreement_score":0.009793244,"about_ca_system_score_codex":0.0022260996,"about_ca_system_score_gemma":0.00077626744,"threshold_uncertainty_score":0.01947248},"labels":[],"label_agreement":null},{"id":"W3001918117","doi":"10.3847/1538-4357/ab6f04","title":"Forming Diverse Super-Earth Systems In Situ","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Planet; Orbital elements; Terrestrial planet; Orbital period; In situ; Planetary system; Transit (satellite); Variation (astronomy)","score_opus":0.015395785509156799,"score_gpt":0.20495435831693945,"score_spread":0.18955857280778265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3001918117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979627,0.00001646975,0.0007095671,0.000033022614,0.0000041623384,0.0000081317085,0.00008195264,0.0000146224265,0.001169412],"genre_scores_gemma":[0.9992065,0.000017953058,0.00040564706,0.0000143840625,0.0000014235062,0.000008828125,0.000108809676,0.000006137627,0.00023032089],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988997,0.000022406764,0.000005317365,0.000030544743,0.000014138536,0.000037530357],"domain_scores_gemma":[0.99944264,0.00022884492,0.00011219001,0.000064142805,0.00005024817,0.00010187076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003004244,0.00028464303,0.00036770766,0.00036598145,0.0005964712,0.0008461476,0.0008358498,0.000707282,0.0027625929],"category_scores_gemma":[0.0016515991,0.00021555528,0.0006474143,0.00034760288,0.0006378523,0.0008784793,0.00088097475,0.00048816905,0.00015164804],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024305482,0.00021039577,0.08854114,0.000050435592,0.0001456574,0.00044604077,0.00038289634,0.8973027,0.004677997,0.0039113276,0.00047558735,0.003612775],"study_design_scores_gemma":[0.000132016,0.00037233715,0.041935798,0.000019853747,0.000083360515,0.00027179628,0.001094196,0.9488312,0.0023123603,0.0030763713,0.0018325215,0.00003816974],"about_ca_topic_score_codex":0.009285043,"about_ca_topic_score_gemma":0.007829556,"teacher_disagreement_score":0.009285043,"about_ca_system_score_codex":0.0008646293,"about_ca_system_score_gemma":0.00038236575,"threshold_uncertainty_score":0.018462002},"labels":[],"label_agreement":null},{"id":"W3003420132","doi":"10.3847/1538-4357/ab72f0","title":"Estimating the Jet Power of Mrk 231 during the 2017–2018 Flare","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Very Long Baseline Array; Blazar; Flare; Quasar; Jet (fluid); Luminosity; Core (optical fiber); Flux (metallurgy)","score_opus":0.010370068401600789,"score_gpt":0.2212488972668221,"score_spread":0.2108788288652213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3003420132","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988238,0.000056887322,0.0001576257,0.00001943801,0.0000043183327,0.000004905287,0.00045238153,0.000030858744,0.0004498673],"genre_scores_gemma":[0.9986235,0.000030755433,0.0001830105,0.000007505061,0.000010878244,0.0000039708875,0.0009921573,0.000008295098,0.0001399555],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998524,0.000008076809,0.000007729306,0.000038850514,0.000038518338,0.00005436081],"domain_scores_gemma":[0.9994941,0.000080009624,0.00019419518,0.000035046745,0.000071171125,0.00012554492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028708854,0.0002879383,0.00027031443,0.0009463572,0.00027702865,0.0006858014,0.00027274244,0.00035276433,0.00073676894],"category_scores_gemma":[0.0009497228,0.00016511897,0.0003450627,0.0003697884,0.00018183685,0.00040471213,0.0003498681,0.00028565899,0.0004019632],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024717662,0.000054579665,0.97852474,0.000023189323,0.000096037635,0.00033074766,0.00013715832,0.0026967193,0.00983718,0.00008788049,0.0005171532,0.007447436],"study_design_scores_gemma":[0.0000040870727,0.000037308262,0.99560094,0.0000033642375,0.000026292008,0.000085066844,0.00006905775,0.003297615,0.0005785489,0.000019212395,0.00027251622,0.000005962511],"about_ca_topic_score_codex":0.007711182,"about_ca_topic_score_gemma":0.008402705,"teacher_disagreement_score":0.007711182,"about_ca_system_score_codex":0.00044002393,"about_ca_system_score_gemma":0.0001381758,"threshold_uncertainty_score":0.01533258},"labels":[],"label_agreement":null},{"id":"W3003548556","doi":"10.3847/1538-4357/ab65f9","title":"AstroSat UVIT Observations of Her X-1","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Light curve; Astrophysics; Neutron star; Telescope; Astronomy; Orbital period; Accretion (finance); Spectral line; X-ray binary; Eclipse; Stars","score_opus":0.03269439389906886,"score_gpt":0.2367166276437799,"score_spread":0.20402223374471104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3003548556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9883233,0.00024113501,0.00039743952,0.000059820097,0.000010582707,0.000012270407,0.0016457496,0.00014846619,0.009161247],"genre_scores_gemma":[0.9926514,0.000108097505,0.0015277265,0.000038426675,0.000025607818,0.0000098560795,0.0035014844,0.00003236909,0.0021051997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998975,0.000013441359,0.0000031453246,0.000032323333,0.000035055607,0.000018592555],"domain_scores_gemma":[0.99985886,0.000011954097,0.000045330704,0.000024118894,0.000025633988,0.00003416201],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026917204,0.00021064392,0.00024829566,0.00089653814,0.00046125046,0.00039567493,0.000231,0.00024175062,0.0015528781],"category_scores_gemma":[0.00024375567,0.00018948257,0.00016572388,0.00071628735,0.00013539678,0.00022332925,0.00048846926,0.000240334,0.0005218019],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014611204,0.00022780972,0.6697327,0.0002707917,0.00026309912,0.0020694607,0.0012332731,0.007522154,0.24382369,0.0037164174,0.010392121,0.059287395],"study_design_scores_gemma":[0.0000590318,0.00024128736,0.96626806,0.000026282183,0.00006188456,0.00066222815,0.00016706633,0.008026885,0.010351091,0.00033768546,0.013781936,0.000016689999],"about_ca_topic_score_codex":0.0027360807,"about_ca_topic_score_gemma":0.0050015794,"teacher_disagreement_score":0.0027360807,"about_ca_system_score_codex":0.00045422194,"about_ca_system_score_gemma":0.00012526415,"threshold_uncertainty_score":0.0054403543},"labels":[],"label_agreement":null},{"id":"W3003828582","doi":"10.3847/1538-4357/ab63cd","title":"The ELM Survey. VIII. Ninety-eight Double White Dwarf Binaries","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration","keywords":"White dwarf; Stars; Sky; Low Mass; Binary star; Gravitational wave","score_opus":0.019767097877524863,"score_gpt":0.2288129330782351,"score_spread":0.20904583520071024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3003828582","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9758623,0.0005049068,0.00033909528,0.00009172676,0.000008872687,0.000035123903,0.01935526,0.00008366054,0.0037189873],"genre_scores_gemma":[0.93813133,0.0004105333,0.0012719386,0.00012782696,0.000028107135,0.00008757346,0.05448253,0.000036295263,0.005423825],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955636,0.000047375448,0.00005175545,0.00009641089,0.0001246169,0.00012349017],"domain_scores_gemma":[0.9994425,0.000056285153,0.00020250726,0.00007883395,0.00007874372,0.0001410347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000509164,0.00025114178,0.00024137796,0.002293074,0.0003354963,0.00053988217,0.00038750307,0.000172296,0.0033854079],"category_scores_gemma":[0.0007309264,0.00015477253,0.00017716427,0.0016394017,0.0001372965,0.00030102677,0.001138675,0.00019202709,0.0021260302],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015932333,0.00003742874,0.9649729,0.000054380645,0.000025663336,0.000152162,0.00024477817,0.000082204475,0.0019736395,0.00017382385,0.00510026,0.027023464],"study_design_scores_gemma":[0.000007831197,0.000018283597,0.99156594,0.000010702529,0.0000069328244,0.0001366656,0.00014811615,0.00014195642,0.0004455302,0.000030929627,0.00748461,0.0000024291496],"about_ca_topic_score_codex":0.005690308,"about_ca_topic_score_gemma":0.010564192,"teacher_disagreement_score":0.005690308,"about_ca_system_score_codex":0.00034692633,"about_ca_system_score_gemma":0.00023482126,"threshold_uncertainty_score":0.0113253},"labels":[],"label_agreement":null},{"id":"W3004414507","doi":"10.3847/1538-4357/ab64f9","title":"High-resolution Near-infrared Polarimetry and Submillimeter Imaging of FS Tau A: Possible Streamers in Misaligned Circumbinary Disk System","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Astronomical Observatory of Japan; National Science Council; National Science Foundation; Korea Astronomy and Space Science Institute; National Institutes of Natural Sciences; Japan Society for the Promotion of Science; Ministry of Education, Culture, Sports, Science and Technology; National Radio Astronomy Observatory","keywords":"Circumbinary planet; Submillimeter Array; Polarimetry; Binary number; Circumstellar disk; Polarization (electrochemistry); Line (geometry)","score_opus":0.00737881392487668,"score_gpt":0.21165946305568922,"score_spread":0.20428064913081254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3004414507","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989386,0.000106112755,0.00035995117,0.00001193739,0.0000035841483,0.0000030545013,0.00012750544,0.000015780288,0.0004335904],"genre_scores_gemma":[0.99929416,0.000025040072,0.00043143876,0.0000050998824,0.000006050718,0.0000015558065,0.00012518448,0.0000022049398,0.0001091489],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995697,0.0000037229756,0.0000023707728,0.000015254086,0.000008769664,0.000012840561],"domain_scores_gemma":[0.9998386,0.000021224378,0.00006472653,0.000014289995,0.000022780294,0.000038413218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111364825,0.00015004,0.00013940166,0.0009775865,0.00030280332,0.00042896776,0.00015813904,0.00017713402,0.00068031147],"category_scores_gemma":[0.00019243784,0.0001229403,0.00011933587,0.00044802783,0.00013300261,0.00026445763,0.00019429151,0.00014347982,0.00017623893],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026080667,0.00009504491,0.79107326,0.000036150606,0.00005756441,0.001191542,0.0003770885,0.0009021303,0.18983805,0.00036342748,0.0003772613,0.015427549],"study_design_scores_gemma":[0.0000034594384,0.000015942642,0.9952976,0.0000022963436,0.000010610067,0.00017697854,0.000086671,0.001504855,0.0025606453,0.00006379533,0.00027402162,0.0000031212555],"about_ca_topic_score_codex":0.001933799,"about_ca_topic_score_gemma":0.0029662764,"teacher_disagreement_score":0.001933799,"about_ca_system_score_codex":0.00017064631,"about_ca_system_score_gemma":0.00008417429,"threshold_uncertainty_score":0.0038450956},"labels":[],"label_agreement":null},{"id":"W3004467934","doi":"10.3847/1538-4357/ab6170","title":"Observations of Extreme ICME Ram Pressure Compressing Mercury’s Dayside Magnetosphere to the Surface","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Aeronautics and Space Administration","keywords":"Physics; Magnetosphere; Ram pressure; Mercury (programming language); Astrophysics; Astronomy; Solar wind; Geophysics; Plasma; Stars; Nuclear physics","score_opus":0.0403031658292211,"score_gpt":0.2286913485294197,"score_spread":0.18838818270019858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3004467934","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947812,0.000103728424,0.00031162077,0.000086105894,0.000015241369,0.000009933508,0.00057927036,0.00009980651,0.0040129516],"genre_scores_gemma":[0.99850744,0.000036392154,0.0004687022,0.00004374962,0.000020925618,0.0000049782584,0.0004954504,0.000015011048,0.00040736084],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992204,0.0000032171508,0.0000015979876,0.000015446727,0.000036523736,0.000021282987],"domain_scores_gemma":[0.9999007,0.00001083315,0.000020847856,0.00001198439,0.000026457534,0.000029097262],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010249416,0.0001948854,0.00020874033,0.0005018069,0.0004128485,0.00027984174,0.00022661513,0.0003918798,0.0010140588],"category_scores_gemma":[0.00016598038,0.00010695435,0.00015100103,0.0004131229,0.00019914458,0.00020210787,0.0005600834,0.00050455955,0.00018904766],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008878314,0.00012567292,0.3680389,0.0001383997,0.00016991177,0.0024847456,0.0014835955,0.0011265576,0.5995827,0.00050696393,0.004206013,0.021248749],"study_design_scores_gemma":[0.000022685532,0.00015247705,0.975496,0.00001238901,0.000026516913,0.000473318,0.0003148422,0.0015257037,0.016696122,0.00011248702,0.0051507284,0.000016829381],"about_ca_topic_score_codex":0.00375803,"about_ca_topic_score_gemma":0.0071428805,"teacher_disagreement_score":0.00375803,"about_ca_system_score_codex":0.0002840588,"about_ca_system_score_gemma":0.00014591168,"threshold_uncertainty_score":0.0074723363},"labels":[],"label_agreement":null},{"id":"W3004804782","doi":"10.3847/1538-4357/ab7bdb","title":"Constraining the Mass of the Emerging Galaxy Cluster SpARCS1049+56 at z = 1.71 with Infrared Weak Lensing","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; York University; McGill University","funders":"","keywords":"Galaxy cluster; Galaxy; Brightest cluster galaxy; Redshift; Cluster (spacecraft); Interacting galaxy; Mass distribution; Weak gravitational lensing; Galaxy formation and evolution","score_opus":0.010546262116879705,"score_gpt":0.2008079655247796,"score_spread":0.1902617034078999,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3004804782","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977062,0.00008096754,0.0008288045,0.000016503089,0.0000051571074,0.000004886042,0.00028319884,0.000037999678,0.001036268],"genre_scores_gemma":[0.99815315,0.000034378227,0.00083216827,0.000012855532,0.000007866347,0.0000026820721,0.00074098865,0.0000068109835,0.00020904263],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998374,0.00001406952,0.000006976857,0.000052917036,0.000050990337,0.000037593534],"domain_scores_gemma":[0.9995302,0.00006565094,0.00013517424,0.00005337852,0.000087740395,0.00012798164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034082035,0.00037349178,0.0003397441,0.0013711257,0.00036108677,0.00052324624,0.0003748451,0.00020260875,0.00092576665],"category_scores_gemma":[0.00047003585,0.00021099005,0.00028890983,0.00054777344,0.00020321799,0.00020607538,0.00053117133,0.00022279097,0.00030982585],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023369852,0.00004694774,0.94490224,0.000030250116,0.00015170085,0.00017578906,0.00006586949,0.005373954,0.037564054,0.0005375033,0.0007619089,0.010155992],"study_design_scores_gemma":[0.000012601717,0.000067575005,0.9728094,0.000010416787,0.00007211504,0.00008161159,0.000092029266,0.018814784,0.006884485,0.0001960348,0.00094707456,0.0000117797],"about_ca_topic_score_codex":0.007930825,"about_ca_topic_score_gemma":0.01466218,"teacher_disagreement_score":0.007930825,"about_ca_system_score_codex":0.00038741925,"about_ca_system_score_gemma":0.00017399382,"threshold_uncertainty_score":0.015769303},"labels":[],"label_agreement":null},{"id":"W3005043992","doi":"10.3847/1538-4357/ab7303","title":"Detection of Strong Epicyclic Density Spikes in the GD-1 Stellar Stream: An Absence of Evidence for the Influence of Dark Matter Subhalos?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Dark matter; Spectrograph; Stars; Astronomy; Photometry (optics); Telescope; Astrometry; Very Large Telescope; Stellar density; Radial velocity; Spectral line","score_opus":0.042822873922705514,"score_gpt":0.27798741775474517,"score_spread":0.23516454383203966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005043992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967294,0.000078628276,0.0011812428,0.00009664427,0.000008340251,0.0000073632928,0.00030790176,0.0000924912,0.0014979311],"genre_scores_gemma":[0.9992853,0.000019485884,0.00034619262,0.000012398993,0.000003871967,0.000001726132,0.00019739424,0.000020323172,0.00011326937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993217,0.000012143375,0.000004394153,0.000021279144,0.000014991249,0.00001500149],"domain_scores_gemma":[0.99974424,0.000043515764,0.00007174078,0.000052169336,0.00003504435,0.000053302392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023520265,0.00015712492,0.00028837653,0.0002809761,0.00024664617,0.0007332433,0.00040877372,0.00022033729,0.0011822489],"category_scores_gemma":[0.0011149909,0.0001351365,0.00021678102,0.00027498585,0.00034195275,0.00022669855,0.00046453686,0.00024586925,0.00032435544],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029309132,0.00005921547,0.9403602,0.00007039384,0.00012865044,0.00066214317,0.00026179216,0.017614635,0.021524692,0.0023297397,0.001442423,0.01525313],"study_design_scores_gemma":[0.000049318427,0.00005999783,0.8598967,0.000021530486,0.000044074925,0.00034066424,0.00017211557,0.13104692,0.004450591,0.0012548817,0.0026491869,0.000013984967],"about_ca_topic_score_codex":0.009690695,"about_ca_topic_score_gemma":0.0085064955,"teacher_disagreement_score":0.009690695,"about_ca_system_score_codex":0.00049804046,"about_ca_system_score_gemma":0.00023398096,"threshold_uncertainty_score":0.019268572},"labels":[],"label_agreement":null},{"id":"W3005330457","doi":"10.3847/1538-4357/abf7c4","title":"Supernova Model Discrimination with Hyper-Kamiokande","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"British Columbia Institute of Technology; University of Toronto; University of Winnipeg; York University; University of British Columbia; University of Victoria; University of Regina; Carleton University; TRIUMF","funders":"Science and Technology Facilities Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Japan Society for the Promotion of Science; Ministry of Science, ICT and Future Planning; Russian Foundation for Basic Research; Ministry of Education, Culture, Sports, Science and Technology; Horizon 2020 Framework Programme; UK Research and Innovation","keywords":"Physics; Supernova; Neutrino; Astrophysics; Astronomy; Type II supernova; Neutrino detector; Accretion (finance); Neutron star; Neutrino oscillation; Particle physics","score_opus":0.011900603525479858,"score_gpt":0.2189413496409708,"score_spread":0.20704074611549095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005330457","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925483,0.000045099234,0.0056919646,0.00006198875,0.00004108585,0.00002166925,0.00020002887,0.0002684446,0.0011214553],"genre_scores_gemma":[0.99676645,0.000016567143,0.0026537704,0.000020114894,0.000004407869,0.000012498154,0.00022984763,0.000029424142,0.00026684313],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998385,0.000048026963,0.000011269837,0.00003931407,0.000031248608,0.000031618016],"domain_scores_gemma":[0.9988695,0.0006322706,0.00012243025,0.00012356593,0.00014894766,0.000103249506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006694031,0.00045909535,0.00038246394,0.00036582988,0.00020990132,0.00062161434,0.00087913446,0.0005661581,0.0015178589],"category_scores_gemma":[0.0020717492,0.00020990291,0.00066360336,0.00020163512,0.00033348758,0.00038975282,0.0005076859,0.0006260883,0.00011766692],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027920082,0.00012913963,0.017759038,0.000031567357,0.00012281527,0.000120044424,0.00004423636,0.97237116,0.0040352964,0.002503356,0.00027996977,0.0023241467],"study_design_scores_gemma":[0.000030074603,0.000053112555,0.0014653502,0.0000018505636,0.000012893901,0.000014762839,0.000006555958,0.99589866,0.0020218368,0.00037402066,0.000114298426,0.000006578329],"about_ca_topic_score_codex":0.00572147,"about_ca_topic_score_gemma":0.0030833492,"teacher_disagreement_score":0.00572147,"about_ca_system_score_codex":0.0005533622,"about_ca_system_score_gemma":0.00043319995,"threshold_uncertainty_score":0.011376381},"labels":[],"label_agreement":null},{"id":"W3005362685","doi":"10.3847/1538-4357/ab5b05","title":"Fermi and Swift Observations of GRB 190114C: Tracing the Evolution of High-energy Emission from Prompt to Afterglow","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council; Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; Agenzia Spaziale Italiana; High Energy Accelerator Research Organization; Bundesministerium für Bildung und Forschung; Japan Society for the Promotion of Science; Israel Science Foundation; University of Leicester; Marshall Space Flight Center; Istituto Nazionale di Astrofisica; Kanazawa University; Universities Space Research Association; Centre National de la Recherche Scientifique; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; U.S. Department of Energy","keywords":"Afterglow; Gamma-ray burst; Fermi Gamma-ray Space Telescope; Lorentz factor; Telescope; Light curve; Emission spectrum; Spitzer Space Telescope; Synchrotron","score_opus":0.015060117321182724,"score_gpt":0.21293334568541855,"score_spread":0.19787322836423582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005362685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983829,0.00013795601,0.0003506781,0.00002347699,0.00000532917,0.00000647259,0.00035055337,0.000043284406,0.00069928414],"genre_scores_gemma":[0.99819046,0.000069356654,0.00069037627,0.00002510703,0.000009944556,0.00000706686,0.00078140514,0.000010097346,0.00021605597],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993503,0.000007071391,0.0000032236576,0.000014376661,0.000018396484,0.000021882708],"domain_scores_gemma":[0.99979347,0.000029206289,0.000072866475,0.000016713577,0.00003932636,0.00004842732],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021341027,0.00026503237,0.00024140673,0.000931336,0.00031192007,0.00035456207,0.0002547576,0.00030914723,0.00066229363],"category_scores_gemma":[0.00036403193,0.00015481134,0.00022342977,0.00043899534,0.00016083848,0.00014792307,0.00032654472,0.00032547585,0.00020773766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057015056,0.00027387138,0.8637181,0.000061429106,0.000099682846,0.00094163854,0.0002970505,0.0013415476,0.10937779,0.00031847536,0.001666783,0.021333534],"study_design_scores_gemma":[0.000009512093,0.000066222055,0.9960632,0.000006811289,0.000016275453,0.00019387329,0.000038185815,0.0009835439,0.0018863227,0.000037009126,0.0006924836,0.0000065648496],"about_ca_topic_score_codex":0.0057980665,"about_ca_topic_score_gemma":0.012731066,"teacher_disagreement_score":0.0057980665,"about_ca_system_score_codex":0.0003240748,"about_ca_system_score_gemma":0.00013548849,"threshold_uncertainty_score":0.011528671},"labels":[],"label_agreement":null},{"id":"W3005448633","doi":"10.3847/1538-4357/ab5303","title":"WISE 2150-7520AB: A Very Low-mass, Wide Comoving Brown Dwarf System Discovered through the Citizen Science Project Backyard Worlds: Planet 9*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Planet; Astrobiology; Citizen science; Astronomy; Dwarf planet; Brown dwarf; Physics","score_opus":0.01625284981097766,"score_gpt":0.22980838495332126,"score_spread":0.2135555351423436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005448633","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9939423,0.00009991121,0.00044205465,0.0000878942,0.000017894652,0.000016843656,0.0009314441,0.000107758024,0.004353758],"genre_scores_gemma":[0.9941401,0.000054529464,0.001340814,0.0001473935,0.000020372325,0.000014089793,0.002127191,0.000029178838,0.0021262753],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998524,0.00000731803,0.0000063523294,0.000037436792,0.000049640264,0.000046870216],"domain_scores_gemma":[0.9996277,0.000013351099,0.00009156387,0.000041819887,0.000044544813,0.0001810732],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016658223,0.00029913028,0.00026037678,0.0010751422,0.0011294025,0.00059882173,0.0003163606,0.0003356263,0.0019380611],"category_scores_gemma":[0.00028826846,0.00014287884,0.00020995093,0.0006551981,0.00041469745,0.00031967592,0.0011372583,0.00028925986,0.0013556508],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000485456,0.00017659033,0.8424602,0.000092907234,0.00012061056,0.006823465,0.0018539736,0.00022013122,0.09392554,0.0015377993,0.010990297,0.04131306],"study_design_scores_gemma":[0.000015909669,0.00018012867,0.9594797,0.000017411092,0.000042127067,0.0037382683,0.00079037884,0.0005362469,0.008701347,0.00036112644,0.026115377,0.000022104825],"about_ca_topic_score_codex":0.006527575,"about_ca_topic_score_gemma":0.013787439,"teacher_disagreement_score":0.006527575,"about_ca_system_score_codex":0.0003646217,"about_ca_system_score_gemma":0.00031614772,"threshold_uncertainty_score":0.01297915},"labels":[],"label_agreement":null},{"id":"W3005478311","doi":"10.3847/1538-4357/ab74dd","title":"A Novel Survey for Young Substellar Objects with the W-band Filter. II. The Coolest and Lowest Mass Members of the Serpens-South Star-forming Region","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Brown dwarf; Photometry (optics); Serpens; Stellar classification; Low Mass; Stars","score_opus":0.022518049339533018,"score_gpt":0.2167896700110709,"score_spread":0.1942716206715379,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005478311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99684733,0.00005497028,0.0015263117,0.000008218642,0.0000025973711,0.000019430914,0.00040705467,0.000054071,0.0010800131],"genre_scores_gemma":[0.99344146,0.000071327464,0.0040340144,0.000018583773,0.000007676041,0.000017137343,0.0014579069,0.00001143837,0.00094029104],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986863,0.000013005736,0.000010002808,0.000049186652,0.000028714405,0.000030440015],"domain_scores_gemma":[0.9997367,0.000019076191,0.00008732806,0.0000421524,0.00004270178,0.000071954986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002319753,0.00019317871,0.00014572799,0.0012691377,0.00026192798,0.00028785624,0.0002405777,0.00014582349,0.0009705469],"category_scores_gemma":[0.00023636717,0.00011039422,0.00019597531,0.00060903234,0.00012551261,0.00027191913,0.00039181573,0.0001256786,0.00043412554],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007947567,0.00006254463,0.8957825,0.000034924353,0.000029766223,0.00021123454,0.0002707679,0.00014516538,0.07271486,0.00011072422,0.0003164716,0.030241452],"study_design_scores_gemma":[0.0000036206245,0.000057711357,0.9916163,0.000004269268,0.000014776353,0.00028681546,0.00017899084,0.00055638177,0.0057050698,0.00003228622,0.0015407926,0.0000029817431],"about_ca_topic_score_codex":0.0022738348,"about_ca_topic_score_gemma":0.0063324855,"teacher_disagreement_score":0.0022738348,"about_ca_system_score_codex":0.00013764505,"about_ca_system_score_gemma":0.00017582436,"threshold_uncertainty_score":0.0045212507},"labels":[],"label_agreement":null},{"id":"W3005623249","doi":"10.3847/1538-4357/ab74df","title":"The Chandra High-resolution X-Ray Spectrum of Quiescent Emission from Sgr A*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Spectral line; Emission spectrum; RADIUS; Line (geometry); Accretion (finance); Galaxy; Ionization; Stars; Active galactic nucleus","score_opus":0.01301196727842827,"score_gpt":0.2139916663215766,"score_spread":0.20097969904314833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005623249","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99429387,0.0001492993,0.0013539891,0.000060690174,0.00001403267,0.000010522059,0.0011925569,0.00051290274,0.0024120829],"genre_scores_gemma":[0.99557686,0.000052084575,0.0021525293,0.000049587718,0.0000124294365,0.0000064197625,0.0017617096,0.00007487637,0.00031339267],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999124,0.000009446231,0.0000068095123,0.000029780986,0.000022665214,0.000018917784],"domain_scores_gemma":[0.9996804,0.000041101273,0.00007430544,0.000057007772,0.00003761044,0.000109491826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021951635,0.0003174325,0.00026852454,0.0007801496,0.00038025738,0.000555705,0.00032431402,0.0002748857,0.0015503288],"category_scores_gemma":[0.00030071064,0.00018339297,0.00038026695,0.00050855457,0.00020062276,0.00022342488,0.0003593548,0.0003730484,0.0004217049],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014398678,0.00041448895,0.41905946,0.0002560384,0.0003944591,0.0019192206,0.0005493459,0.0077426843,0.520068,0.0023271334,0.008968743,0.03686046],"study_design_scores_gemma":[0.000027844493,0.00017132543,0.9719296,0.000011640145,0.000043858665,0.00080133195,0.000094323805,0.00956887,0.014324446,0.00029980132,0.0027074334,0.000019480975],"about_ca_topic_score_codex":0.0017991678,"about_ca_topic_score_gemma":0.002619142,"teacher_disagreement_score":0.0017991678,"about_ca_system_score_codex":0.00022612563,"about_ca_system_score_gemma":0.00011297747,"threshold_uncertainty_score":0.0051863194},"labels":[],"label_agreement":null},{"id":"W3005815659","doi":"10.3847/1538-4357/abd407","title":"An Improved Measurement of the Secondary Cosmic Microwave Background Anisotropies from the SPT-SZ + SPTpol Surveys","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of Colorado Boulder; Office of Science; Argonne National Laboratory; National Energy Research Scientific Computing Center; McGill University; Gordon and Betty Moore Foundation; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Cosmic microwave background; Reionization; Multipole expansion; Spectral density; Cosmic infrared background; Spectral line; Anisotropy; Cosmic background radiation","score_opus":0.015615589697841012,"score_gpt":0.2404956955058436,"score_spread":0.22488010580800258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3005815659","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97866654,0.00016405199,0.009863845,0.0001396717,0.000028622895,0.000025248995,0.003321844,0.00017914118,0.0076110642],"genre_scores_gemma":[0.99092054,0.00008495844,0.004839051,0.000030813015,0.00004814695,0.000016463884,0.0036818474,0.000038173883,0.0003400079],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99922407,0.00012584911,0.00003286341,0.00023275762,0.0002895605,0.00009483695],"domain_scores_gemma":[0.9977829,0.00028589775,0.00067839253,0.00050785666,0.00045905093,0.0002860038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008790876,0.0005274591,0.0002864963,0.0015680514,0.00022569527,0.0008920621,0.0004149009,0.00024636646,0.0016413508],"category_scores_gemma":[0.0028031068,0.00033414224,0.00039336554,0.001775008,0.00026228733,0.0005821671,0.0010427426,0.00066256226,0.0004877546],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005946503,0.0000685223,0.87817574,0.00013361315,0.0003357673,0.00033366133,0.0002534594,0.0044603776,0.044761963,0.0019375209,0.0033188858,0.06562583],"study_design_scores_gemma":[0.000029045133,0.00006996089,0.9853019,0.000009450227,0.00006420671,0.00021242084,0.000029548199,0.0042047314,0.005635147,0.00039299772,0.0040364596,0.000014173651],"about_ca_topic_score_codex":0.0027757091,"about_ca_topic_score_gemma":0.0045728115,"teacher_disagreement_score":0.0027757091,"about_ca_system_score_codex":0.00037552108,"about_ca_system_score_gemma":0.00025427225,"threshold_uncertainty_score":0.0055191517},"labels":[],"label_agreement":null},{"id":"W3006094170","doi":"10.3847/1538-4357/ab64e9","title":"The Strikingly Metal-rich Halo of the Sombrero Galaxy*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Metallicity; Astronomy; Galaxy; Halo; Galactic halo; Context (archaeology); Bulge","score_opus":0.010090227756065506,"score_gpt":0.20504949930988914,"score_spread":0.19495927155382364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3006094170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955171,0.000088734145,0.00024203488,0.000030323903,0.0000023867797,0.000001643087,0.00013462908,0.000026713627,0.003956501],"genre_scores_gemma":[0.9988141,0.00004146656,0.00035472136,0.000021334634,0.000007321873,7.1944123e-7,0.00018964951,0.000005639557,0.00056508335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999449,0.0000035925318,0.0000020707166,0.000021793456,0.00001079586,0.000016835553],"domain_scores_gemma":[0.9997981,0.000014010882,0.00007414549,0.00003242561,0.000018888022,0.00006254941],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009871018,0.00015880511,0.00016013638,0.0005181911,0.00034316292,0.000595673,0.0001578781,0.00018823394,0.0024911372],"category_scores_gemma":[0.00017442321,0.000093505114,0.00011789807,0.0002871469,0.00040870433,0.00027341858,0.00050781225,0.00013852632,0.0005633665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032583287,0.00005346913,0.83685887,0.00009881457,0.0000852711,0.0005704753,0.0006115951,0.0008614532,0.13319625,0.0016004678,0.00072553323,0.02501182],"study_design_scores_gemma":[0.000005553572,0.00004686124,0.9929917,0.0000133788835,0.000008322157,0.0003891074,0.00026672086,0.0005106627,0.0026570486,0.00026072402,0.0028442713,0.0000057754514],"about_ca_topic_score_codex":0.0029000565,"about_ca_topic_score_gemma":0.0061283694,"teacher_disagreement_score":0.0029000565,"about_ca_system_score_codex":0.00022921739,"about_ca_system_score_gemma":0.000074417505,"threshold_uncertainty_score":0.008333743},"labels":[],"label_agreement":null},{"id":"W3006148284","doi":"10.3847/1538-4357/ab744c","title":"Spacetime Tomography Using the Event Horizon Telescope","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Ministero dello Sviluppo Economico; Government of Canada; Ministère de l'Économie, de la Science et de l'Innovation - Québec; Compute Canada; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada; Natural Sciences and Engineering Research Council of Canada; Université de Sherbrooke","keywords":"Event horizon; Supermassive black hole; Sagittarius A*; Accretion (finance); Galactic Center; Spacetime; Accretion disc; General relativity","score_opus":0.01959985474535114,"score_gpt":0.243057681552268,"score_spread":0.22345782680691686,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3006148284","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.29314917,0.00043349434,0.68691915,0.0005285048,0.00007437324,0.000084231484,0.0029211866,0.0022176576,0.013672275],"genre_scores_gemma":[0.7964654,0.00014862302,0.20111437,0.000059131966,0.000034808,0.000026705759,0.0011189424,0.00005673307,0.0009752216],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9997503,0.00010044616,0.000010555172,0.00005420137,0.00005856258,0.000025962216],"domain_scores_gemma":[0.9993218,0.00014282766,0.00019142243,0.00016684731,0.00011262258,0.00006447652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062649685,0.0003192395,0.00020283122,0.0008538927,0.00019645743,0.0004324144,0.000387761,0.0003086819,0.0020355587],"category_scores_gemma":[0.0018431373,0.00023698952,0.000299197,0.0009115422,0.00030366916,0.0007963284,0.0009078801,0.0003859784,0.00026242065],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011749773,0.00016309669,0.11012352,0.00027911522,0.0005162133,0.0019906852,0.0004944009,0.33786625,0.23343122,0.092462786,0.006412471,0.21508525],"study_design_scores_gemma":[0.00006842963,0.00012381733,0.049441256,0.000024251562,0.000051197494,0.0008664637,0.000093710245,0.9034057,0.014714566,0.024312885,0.006836522,0.000061115585],"about_ca_topic_score_codex":0.0030457305,"about_ca_topic_score_gemma":0.0035018008,"teacher_disagreement_score":0.0030457305,"about_ca_system_score_codex":0.00051174255,"about_ca_system_score_gemma":0.0005299551,"threshold_uncertainty_score":0.0068095922},"labels":[],"label_agreement":null},{"id":"W3006258397","doi":"10.3847/1538-4357/ab765d","title":"A Decade of Multiwavelength Observations of the TeV Blazar 1ES 1215+303: Extreme Shift of the Synchrotron Peak Frequency and Long-term Optical–Gamma-Ray Flux Increase","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Office of Science; Sorbonne Université; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; National Science Foundation; Agenzia Spaziale Italiana; Japan Aerospace Exploration Agency; U.S. Department of Energy; California Institute of Technology; European Commission; National Energy Research Scientific Computing Center; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Alexander von Humboldt-Stiftung; Russian Foundation for Basic Research; Jet Propulsion Laboratory; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration","keywords":"Blazar; Synchrotron; Flux (metallurgy); Extreme ultraviolet; Polarization (electrochemistry); Synchrotron radiation; Broadband; Active galactic nucleus","score_opus":0.02123871606446868,"score_gpt":0.22231064089373834,"score_spread":0.20107192482926967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3006258397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99210316,0.0021131362,0.00078626163,0.00025966403,0.000021943812,0.00000783364,0.0008095992,0.000104166225,0.0037941046],"genre_scores_gemma":[0.99633694,0.0007525942,0.0008141241,0.000104091174,0.0000702854,0.0000070450183,0.0012842492,0.000022466189,0.00060828775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985135,0.000011652197,0.000011337768,0.000053173095,0.00004922423,0.00002331534],"domain_scores_gemma":[0.9995598,0.00005391428,0.00022056335,0.000042041855,0.000043609343,0.00008009597],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040460104,0.000241558,0.00021589857,0.001107108,0.00034931587,0.00072279363,0.00021135005,0.00034080667,0.000782467],"category_scores_gemma":[0.00030340208,0.00018623163,0.000176346,0.0009335539,0.0002510503,0.00049178774,0.00071187556,0.0004159525,0.0001574639],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053225737,0.00021829552,0.76196533,0.0003507638,0.00034304443,0.0011101938,0.0007970251,0.0020921058,0.123490684,0.001592574,0.0047978284,0.10270984],"study_design_scores_gemma":[0.00000670284,0.000030187084,0.99434835,0.000016690967,0.000023635008,0.00027424085,0.00005595924,0.00033179123,0.0015683841,0.00010771757,0.0032288888,0.0000074747277],"about_ca_topic_score_codex":0.0015447175,"about_ca_topic_score_gemma":0.0045513217,"teacher_disagreement_score":0.0015447175,"about_ca_system_score_codex":0.00039661129,"about_ca_system_score_gemma":0.00014248837,"threshold_uncertainty_score":0.0030714273},"labels":[],"label_agreement":null},{"id":"W3006978184","doi":"10.3847/1538-4357/ab6c69","title":"Distribution Functions of Energetic Particles Experiencing Compound Subdiffusion","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Distribution (mathematics); Statistical physics; Astrophysics; Astronomy","score_opus":0.010809257727215225,"score_gpt":0.21607064726604489,"score_spread":0.20526138953882966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3006978184","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97418445,0.000073288145,0.022364205,0.00007940307,0.000007904242,0.00001718388,0.000116134266,0.0001079158,0.003049555],"genre_scores_gemma":[0.9979929,0.000034936147,0.0011697386,0.000007192876,0.0000033501763,0.000008102716,0.00008804408,0.00002341756,0.0006724429],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989235,0.000018599303,0.000005745828,0.000019486997,0.000024337849,0.000039473347],"domain_scores_gemma":[0.9986205,0.00059528666,0.00022825011,0.00011351779,0.00024375174,0.00019871682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006023883,0.00034469098,0.00032867354,0.0011431478,0.0005383857,0.0009993322,0.00064352155,0.00039590697,0.0027137876],"category_scores_gemma":[0.0028079813,0.00020479629,0.00029026793,0.0004119514,0.0007950705,0.00084365025,0.00061150495,0.00042996198,0.00025967616],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010609641,0.00020153789,0.053246107,0.0001263361,0.00010769146,0.002108401,0.0011252078,0.7114525,0.07238132,0.13716178,0.0017449985,0.019283175],"study_design_scores_gemma":[0.000014136032,0.00005697832,0.009383917,0.00000832968,0.000006791624,0.00020367528,0.00012903615,0.97603875,0.0059670187,0.007646657,0.0005157954,0.000028908988],"about_ca_topic_score_codex":0.0021079779,"about_ca_topic_score_gemma":0.00072127196,"teacher_disagreement_score":0.0027137876,"about_ca_system_score_codex":0.0009704941,"about_ca_system_score_gemma":0.00031648244,"threshold_uncertainty_score":0.009078562},"labels":[],"label_agreement":null},{"id":"W3007048582","doi":"10.3847/1538-4357/ab339f","title":"The Next Generation Virgo Cluster Survey (NGVS). XIV. The Discovery of Low-mass Galaxies and a New Galaxy Catalog in the Core of the Virgo Cluster<sup>∗</sup>","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Waterloo; Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Virgo Cluster; Physics; Astrophysics; Galaxy; Astronomy; Galaxy cluster; Sky; Population; Surface brightness","score_opus":0.02783415574444932,"score_gpt":0.22515851431478104,"score_spread":0.1973243585703317,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007048582","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7670505,0.0015989448,0.0021747793,0.00090731075,0.00008156678,0.00015349765,0.20037362,0.00070536433,0.02695434],"genre_scores_gemma":[0.59747505,0.0008386789,0.004548663,0.0003243145,0.00007803563,0.00015195271,0.37987122,0.00008560906,0.016626516],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984264,0.000017242075,0.000006001475,0.00003092592,0.00006843831,0.000034810524],"domain_scores_gemma":[0.9996921,0.000029468405,0.000060283928,0.000051425093,0.000072029354,0.00009479165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034578782,0.00014659305,0.00012418946,0.0012743585,0.00020205582,0.0004458714,0.0003054954,0.00017960451,0.0032229589],"category_scores_gemma":[0.0006025812,0.00011122665,0.00012360231,0.0013382611,0.00013476255,0.00017238785,0.0005654551,0.0001596814,0.001607345],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002691549,0.000049952305,0.77044797,0.00016571039,0.00007675275,0.00015962968,0.00031750512,0.0016423739,0.0047291867,0.0032123171,0.11738802,0.10154147],"study_design_scores_gemma":[0.000016467182,0.000020722186,0.9419303,0.000022272192,0.0000147755645,0.000059004713,0.00008170318,0.0010670464,0.00081199413,0.00029826644,0.05567126,0.000006164566],"about_ca_topic_score_codex":0.037131984,"about_ca_topic_score_gemma":0.038329538,"teacher_disagreement_score":0.037131984,"about_ca_system_score_codex":0.00066724233,"about_ca_system_score_gemma":0.0004179916,"threshold_uncertainty_score":0.07383174},"labels":[],"label_agreement":null},{"id":"W3007121356","doi":"10.3847/1538-4357/ab7378","title":"Velocity-coherent Filaments in NGC 1333: Evidence for Accretion Flow?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics; University of Alberta; University of Victoria","funders":"","keywords":"Protein filament; Velocity gradient; Accretion (finance); Scale (ratio); Length scale; Falling (accident); Flow (mathematics)","score_opus":0.05160506722528884,"score_gpt":0.3013108023440586,"score_spread":0.24970573511876976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007121356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954899,0.0001577516,0.001390161,0.00009333263,0.0000072958624,0.0000073513247,0.00051956205,0.00022339853,0.0021114098],"genre_scores_gemma":[0.9987154,0.000030689087,0.00078098517,0.000020312045,0.000007071581,0.0000032578369,0.0002883827,0.000017994136,0.00013596004],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999361,0.0000044797653,0.0000029560008,0.00002095414,0.000015398673,0.00002008578],"domain_scores_gemma":[0.9996915,0.000035418565,0.0001355679,0.000030288487,0.00003530276,0.00007191886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001298929,0.00016844609,0.0001449855,0.0006749301,0.00035509502,0.00058099336,0.0002425164,0.0003205659,0.0017657108],"category_scores_gemma":[0.00048297655,0.00016745512,0.00012800648,0.0006363513,0.00032296905,0.0002697861,0.00037162236,0.0002482701,0.0003097777],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034016056,0.000086294196,0.77039564,0.00008862032,0.000088222136,0.0011267895,0.00067379803,0.002279688,0.19954085,0.0012023806,0.002097875,0.022079686],"study_design_scores_gemma":[0.000010751032,0.000023166707,0.9926496,0.000015360685,0.000013688329,0.00021969061,0.00016413459,0.00331287,0.0021498108,0.00038338063,0.0010496237,0.000007881083],"about_ca_topic_score_codex":0.007697756,"about_ca_topic_score_gemma":0.011018975,"teacher_disagreement_score":0.007697756,"about_ca_system_score_codex":0.00031172953,"about_ca_system_score_gemma":0.00017596272,"threshold_uncertainty_score":0.015305936},"labels":[],"label_agreement":null},{"id":"W3007320440","doi":"10.3847/1538-4357/ab75ee","title":"LATIS: The Lyα Tomography IMACS Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Galaxy; Astrophysics; QSOS; Universe; Opacity; Telescope; Spectral line; Intergalactic medium; Dark matter; Astronomy; Redshift; Optics","score_opus":0.012853558051959691,"score_gpt":0.21350416615495532,"score_spread":0.20065060810299562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007320440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.46296403,0.0009166306,0.033182584,0.0030953742,0.00022654026,0.0011474263,0.35722685,0.017461922,0.1237787],"genre_scores_gemma":[0.5582739,0.0006198923,0.05406105,0.0011349551,0.0005265709,0.0010583749,0.3585776,0.0010994163,0.024648188],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99946076,0.00009251339,0.000022116144,0.00011902666,0.00021566247,0.00008993142],"domain_scores_gemma":[0.9989698,0.000052279876,0.00019659764,0.00018089624,0.00035277664,0.0002476816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00073817564,0.0005226646,0.0002683127,0.0024450074,0.00056540605,0.0009889073,0.00093415764,0.00033809853,0.007546845],"category_scores_gemma":[0.0011957888,0.00022809266,0.00019926044,0.002246207,0.0001811557,0.0008417976,0.0013478717,0.00047216372,0.0048591536],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007993717,0.00026946058,0.35253888,0.00023661934,0.00015726755,0.0007138062,0.0009958071,0.0077320314,0.014969228,0.009694343,0.4238621,0.1880311],"study_design_scores_gemma":[0.00019129449,0.00015792463,0.4523848,0.00012276752,0.00007779652,0.0007333444,0.0008191776,0.027656052,0.010799988,0.0037974746,0.50316334,0.00009605471],"about_ca_topic_score_codex":0.01754411,"about_ca_topic_score_gemma":0.023084829,"teacher_disagreement_score":0.01754411,"about_ca_system_score_codex":0.0009735957,"about_ca_system_score_gemma":0.0008035815,"threshold_uncertainty_score":0.034883976},"labels":[],"label_agreement":null},{"id":"W3007402826","doi":"10.3847/1538-4357/ab612c","title":"Water in the Star-forming Region NGC 7129 FIRS 2","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Envelope (radar); Circumstellar envelope; Stars; Star formation; RADIUS; Astronomy; Spectral line; Radiative transfer; Line (geometry); Space observatory; Infrared; Optics; Geometry","score_opus":0.019319398574253105,"score_gpt":0.23157170204241265,"score_spread":0.21225230346815954,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3007402826","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993736,0.000021939213,0.000076050725,0.000008871245,6.97661e-7,0.0000023222415,0.000096897704,0.000010462975,0.0004090561],"genre_scores_gemma":[0.9995617,0.000012863658,0.00010133116,0.0000064069404,0.0000010055082,0.0000015374765,0.0001837751,0.0000027409528,0.0001285242],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999503,0.0000033106642,0.0000017295079,0.000017415747,0.000010855313,0.000016336633],"domain_scores_gemma":[0.9999292,0.0000064883916,0.000020841591,0.0000056785166,0.000010150921,0.000027643318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000094505944,0.00025908067,0.00023940961,0.00036029762,0.00050700165,0.0003141572,0.000284477,0.00023308428,0.0008269212],"category_scores_gemma":[0.000117707874,0.00016645601,0.00013400601,0.00020033297,0.00022805395,0.00019198956,0.00027876327,0.00015348627,0.0001764037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003200132,0.00015280819,0.78118074,0.00004771956,0.00005927388,0.001171272,0.00062820734,0.008995249,0.19914432,0.00054129405,0.00067629985,0.0070828246],"study_design_scores_gemma":[0.000022109438,0.00007470687,0.98723745,0.0000056903705,0.0000153054,0.00015882037,0.00022557734,0.007752596,0.003734818,0.00011872974,0.00064504636,0.00000906866],"about_ca_topic_score_codex":0.03308829,"about_ca_topic_score_gemma":0.05073487,"teacher_disagreement_score":0.03308829,"about_ca_system_score_codex":0.0007045859,"about_ca_system_score_gemma":0.00023515377,"threshold_uncertainty_score":0.06579143},"labels":[],"label_agreement":null},{"id":"W3008154247","doi":"10.3847/1538-4357/ab77ab","title":"Properties of Trans-fast Magnetosonic Jets in Black Hole Magnetospheres","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Black hole (networking); Inflow; Magnetohydrodynamics; Magnetosphere; Jet (fluid); Magnetohydrodynamic drive; Outflow; Astrophysical jet; Rotating black hole; Magnetic field; Computational physics; Mechanics; Active galactic nucleus; Astrophysics; Accretion (finance)","score_opus":0.014186556816794052,"score_gpt":0.20136464834528975,"score_spread":0.18717809152849568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3008154247","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9735146,0.0003189928,0.021840982,0.00015881922,0.000031773903,0.000018130972,0.00008994027,0.00014256271,0.003884138],"genre_scores_gemma":[0.9987754,0.0000556691,0.00081414916,0.000007744262,0.000011106766,0.0000031333032,0.000036935024,0.0000116942,0.00028418208],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999385,0.000017938268,0.0000036804322,0.000009304424,0.000012190724,0.000018405586],"domain_scores_gemma":[0.99968946,0.00006014056,0.000117410855,0.000028090437,0.00005326228,0.000051734365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031887266,0.000578838,0.00023684677,0.00057771034,0.00033200457,0.00072295935,0.00035097654,0.0003908747,0.0009855157],"category_scores_gemma":[0.0011299067,0.00020500063,0.00045197815,0.00022409072,0.0005770334,0.0006369936,0.0005513852,0.000297622,0.000102162194],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009678475,0.00013874877,0.12203083,0.00022306287,0.00022456625,0.0036516064,0.0010025235,0.58364004,0.13767341,0.12660988,0.0018724353,0.021965057],"study_design_scores_gemma":[0.000071496484,0.00019359359,0.027398454,0.00001566623,0.000026899797,0.00035197372,0.0001502766,0.94776744,0.0064721615,0.01676819,0.000756208,0.000027624086],"about_ca_topic_score_codex":0.0012699122,"about_ca_topic_score_gemma":0.00042200898,"teacher_disagreement_score":0.0012699122,"about_ca_system_score_codex":0.00036329712,"about_ca_system_score_gemma":0.00016006097,"threshold_uncertainty_score":0.003296852},"labels":[],"label_agreement":null},{"id":"W3008417309","doi":"10.3847/1538-4357/ab6612","title":"The Great Markarian 421 Flare of 2010 February: Multiwavelength Variability and Correlation Studies","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Office of Science; Instituto de Astrofísica de Canarias; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Max-Planck-Gesellschaft; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Nuclear Safety and Security Commission; Japan Society for the Promotion of Science; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Aalto-Yliopisto; Hrvatska Zaklada za Znanost; National Research Centre; European Regional Development Fund; Bundesministerium für Bildung und Forschung; National Energy Research Scientific Computing Center; Deutsche Forschungsgemeinschaft; Russian Foundation for Basic Research; Ministry of Education, Culture, Sports, Science and Technology; Shota Rustaveli National Science Foundation; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Smithsonian Institution; U.S. Department of Energy; Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Blazar; Flare; Astrophysics; Fermi Gamma-ray Space Telescope; Light curve; Flux (metallurgy); Gamma ray; Crab Nebula; Astronomy; MAGIC (telescope)","score_opus":0.014902928070299403,"score_gpt":0.23120517293518744,"score_spread":0.21630224486488803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3008417309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986015,0.000079211015,0.00013616511,0.000030360992,0.000003323754,0.0000052683067,0.00045746102,0.000015981506,0.0006707202],"genre_scores_gemma":[0.9982895,0.00003821121,0.00015420957,0.0000159003,0.000018973575,0.0000053909707,0.0012868936,0.000008204404,0.00018270728],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967384,0.000039224393,0.000018076107,0.00008953175,0.00009265268,0.00008671527],"domain_scores_gemma":[0.9987078,0.0002059799,0.00058562605,0.00012136519,0.0001834135,0.00019576024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042761164,0.00023048256,0.0002989649,0.0014989482,0.00040467025,0.000693899,0.00029777046,0.0002591281,0.0006580957],"category_scores_gemma":[0.0012560018,0.0001478699,0.00025207302,0.0014247192,0.00022398689,0.00024379216,0.00054104923,0.00032707627,0.00029788885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022848934,0.000112263595,0.98304313,0.000017213357,0.00011992732,0.00022561727,0.00026719636,0.0005047718,0.0064813956,0.000086826236,0.00078157696,0.008131659],"study_design_scores_gemma":[0.0000016246984,0.000013053206,0.99927217,0.0000011025513,0.0000043683503,0.000056223467,0.000026210753,0.00031134367,0.00010867164,0.000007630623,0.00019454889,0.0000030869487],"about_ca_topic_score_codex":0.011578017,"about_ca_topic_score_gemma":0.018650344,"teacher_disagreement_score":0.011578017,"about_ca_system_score_codex":0.00041591027,"about_ca_system_score_gemma":0.00017448426,"threshold_uncertainty_score":0.02302128},"labels":[],"label_agreement":null},{"id":"W3008423546","doi":"10.3847/1538-4357/ab76cf","title":"ZFIRE: Measuring Electron Density with [O ii] as a Function of Environment at z = 1.62","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy; Redshift; Electron density; Electron; Cluster (spacecraft); Star formation; Field (mathematics)","score_opus":0.0073440918501357375,"score_gpt":0.167974701427475,"score_spread":0.16063060957733927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3008423546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972493,0.00007174228,0.00047888362,0.000016716496,0.0000018515877,0.000006148196,0.00077453477,0.000071938426,0.0013288992],"genre_scores_gemma":[0.99698573,0.000040426134,0.0012600867,0.000031307343,0.0000044400545,0.00000754707,0.001121088,0.0000092805585,0.0005402162],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991834,0.000008821852,0.000003382079,0.000027513175,0.000021616004,0.000020441199],"domain_scores_gemma":[0.99965405,0.000054609496,0.0001079913,0.00003273929,0.00005556276,0.00009514796],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021788238,0.00019472455,0.00017296511,0.00070682477,0.0002054366,0.00033139298,0.0002225394,0.00018743641,0.0016430606],"category_scores_gemma":[0.0004919469,0.0001282523,0.00009893021,0.0003761056,0.00012042023,0.00023434285,0.00037711213,0.00016283854,0.00032608522],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022159684,0.000040692008,0.9377993,0.000027886748,0.00004809505,0.000077852674,0.00016327843,0.0002669832,0.050057217,0.00012608989,0.0005842365,0.01058674],"study_design_scores_gemma":[0.0000019566091,0.000017545162,0.9978746,0.0000012362063,0.0000041354315,0.000040914427,0.000025675507,0.00017150019,0.001682401,0.000022819895,0.00015576421,0.0000015604952],"about_ca_topic_score_codex":0.0025423309,"about_ca_topic_score_gemma":0.005890345,"teacher_disagreement_score":0.0025423309,"about_ca_system_score_codex":0.00015438398,"about_ca_system_score_gemma":0.000040185063,"threshold_uncertainty_score":0.0054965615},"labels":[],"label_agreement":null},{"id":"W3008668456","doi":"10.3847/1538-4357/ab7b63","title":"Dust-depleted Inner Disks in a Large Sample of Transition Disks through Long-baseline ALMA Observations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":177,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Planet; Protoplanetary disk; Accretion (finance); Debris disk; Submillimeter Array; RADIUS; Astronomy; Millimeter; Thick disk; Planetary system; Angular momentum; Thin disk; Stars; Star formation; Galaxy; Halo","score_opus":0.035378428681783196,"score_gpt":0.2674202302799697,"score_spread":0.2320418015981865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3008668456","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997327,0.000028262017,0.000033747427,0.0000042621355,3.8696663e-7,0.0000024235774,0.00012683032,0.000003170711,0.000068276815],"genre_scores_gemma":[0.9994435,0.00002948477,0.000096864744,0.0000068671307,0.0000030417598,0.0000037917134,0.00033676683,0.0000018232128,0.000077767196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997516,0.000028397802,0.000017650213,0.00009059279,0.000041768628,0.000070002876],"domain_scores_gemma":[0.9993992,0.000084104875,0.0001916612,0.00008803732,0.00008351772,0.00015344101],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023799967,0.00022960038,0.00029764048,0.0010698059,0.00051439804,0.00072103826,0.00033070368,0.00019731293,0.0005226543],"category_scores_gemma":[0.00069335103,0.00020942932,0.00015840934,0.00064524636,0.00024541534,0.00048054243,0.00072181795,0.0002208764,0.00019239179],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009800946,0.00005222164,0.9900557,0.000007029894,0.00003054602,0.00013748652,0.00042972842,0.00004064319,0.006074347,0.000019707217,0.00009177717,0.0029627997],"study_design_scores_gemma":[0.000004086874,0.00003197557,0.9987362,0.0000018258276,0.000014095204,0.00019146301,0.0002705193,0.00014400354,0.00034443036,0.000012219317,0.00024748532,0.0000016729396],"about_ca_topic_score_codex":0.0057791644,"about_ca_topic_score_gemma":0.010736971,"teacher_disagreement_score":0.0057791644,"about_ca_system_score_codex":0.00024998217,"about_ca_system_score_gemma":0.00013504388,"threshold_uncertainty_score":0.01149106},"labels":[],"label_agreement":null},{"id":"W3008838182","doi":"10.3847/1538-4357/ab68db","title":"The NANOGrav 11 yr Data Set: Evolution of Gravitational-wave Background Statistics","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"National Science Foundation","keywords":"Spurious relationship; Noise (video); Gravitational wave; Observatory; Millisecond pulsar; Spectral density; Gravitational wave background; Supermassive black hole; Fourier analysis","score_opus":0.05738732979250499,"score_gpt":0.34430640620015646,"score_spread":0.28691907640765146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3008838182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9914398,0.00007646529,0.0011867116,0.00015551905,0.00002081153,0.000011557939,0.0060971063,0.00015946632,0.00085252407],"genre_scores_gemma":[0.9695916,0.0000373804,0.0015980335,0.000045453195,0.000019708234,0.000014208948,0.028276935,0.00005988161,0.0003566482],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999458,0.0000980233,0.00003882245,0.00018659033,0.00016302364,0.000055545876],"domain_scores_gemma":[0.9979961,0.0008296199,0.00033338083,0.00041509347,0.00025580413,0.00017006103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014767577,0.00033846084,0.0003691238,0.0013192011,0.0002831959,0.0007464432,0.0005792243,0.00044106095,0.0005983185],"category_scores_gemma":[0.0035524634,0.00017471,0.00034957487,0.00097511016,0.00030138026,0.00058951776,0.0007369017,0.0004660559,0.000300165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096954615,0.0002352322,0.8568412,0.00009119008,0.0003193348,0.00047810722,0.00027544476,0.08112081,0.0126625355,0.0027928054,0.009364104,0.034849662],"study_design_scores_gemma":[0.000086258035,0.00015255556,0.72069925,0.000024197238,0.00006144217,0.0003648962,0.00018281266,0.26411158,0.006113683,0.0010045496,0.007149856,0.000048885497],"about_ca_topic_score_codex":0.010910501,"about_ca_topic_score_gemma":0.013768708,"teacher_disagreement_score":0.010910501,"about_ca_system_score_codex":0.0005671862,"about_ca_system_score_gemma":0.00032216794,"threshold_uncertainty_score":0.021694005},"labels":[],"label_agreement":null},{"id":"W3009374067","doi":"10.3847/1538-4357/ab7b6d","title":"MOSEL Survey: Tracking the Growth of Massive Galaxies at 2 &lt; z &lt; 4 Using Kinematics and the IllustrisTNG Simulation","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy; Stellar mass; Velocity dispersion; Star formation; Kinematics; Luminous infrared galaxy; Galaxy formation and evolution; Peculiar galaxy","score_opus":0.02378064743259177,"score_gpt":0.2355280233587451,"score_spread":0.21174737592615334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009374067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911805,0.000051527888,0.00089722493,0.00011838779,0.000005193631,0.000014435436,0.005134906,0.0004887343,0.002109234],"genre_scores_gemma":[0.98670954,0.00004809351,0.0026317541,0.000040163402,0.000011352856,0.000021008495,0.009427345,0.00008643344,0.001024132],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998994,0.000023712164,0.000003030766,0.00003348639,0.000018961102,0.000021477714],"domain_scores_gemma":[0.9995433,0.000076214885,0.000115710754,0.000066094886,0.00007370885,0.00012494528],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045869075,0.00029350293,0.00022712543,0.00074860273,0.00020711584,0.00045294323,0.0005868378,0.00030241327,0.0015841599],"category_scores_gemma":[0.0012587149,0.0001758366,0.00040723404,0.0004951462,0.00016820003,0.00030549802,0.00053678267,0.00030533233,0.00065338484],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036903465,0.00016899843,0.8421746,0.000049334394,0.00030925294,0.000290865,0.00024439878,0.12640715,0.0040830593,0.0021324882,0.008439075,0.015331806],"study_design_scores_gemma":[0.00011201166,0.00012504637,0.59224373,0.000013166398,0.000063017076,0.000065819746,0.00013278013,0.39908436,0.0020449853,0.0005380853,0.0055390075,0.000037980735],"about_ca_topic_score_codex":0.048043244,"about_ca_topic_score_gemma":0.06089491,"teacher_disagreement_score":0.048043244,"about_ca_system_score_codex":0.0007862947,"about_ca_system_score_gemma":0.0002760076,"threshold_uncertainty_score":0.09552723},"labels":[],"label_agreement":null},{"id":"W3009396936","doi":"10.3847/1538-4357/ab700a","title":"Large-scale Molecular Gas Distribution in the M17 Cloud Complex: Dense Gas Conditions of Massive Star Formation?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Protostar; Star formation; Molecular cloud; Gravitational collapse; Stellar evolution; Gravitational potential; Star cluster","score_opus":0.013272887246294496,"score_gpt":0.2497655689001133,"score_spread":0.23649268165381881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009396936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995227,0.00010872221,0.00005469639,0.000010233812,6.3274166e-7,0.0000022995735,0.00006924546,0.0000025591899,0.00022897501],"genre_scores_gemma":[0.99973494,0.00003583028,0.00007090113,0.0000064511137,0.0000028818167,0.0000014582097,0.000106953026,0.0000018541186,0.000038704613],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998766,0.0000073789392,0.0000073332976,0.00003055716,0.000028375905,0.00004966959],"domain_scores_gemma":[0.99954444,0.00003618763,0.0001901585,0.000027714364,0.000051051527,0.00015045087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010406467,0.00017936886,0.0002490748,0.0012351677,0.00041792807,0.000663933,0.00032737106,0.00019795436,0.0010973488],"category_scores_gemma":[0.00036962537,0.00011362658,0.00012057098,0.0007328923,0.0005286071,0.00032943903,0.0006031449,0.0001532631,0.00016603689],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009541098,0.000020245898,0.9615125,0.000019150579,0.000023434775,0.00032345092,0.00014860556,0.00012403559,0.03594072,0.00013223065,0.00005602924,0.0016041681],"study_design_scores_gemma":[0.0000033912079,0.000029234918,0.9970174,0.0000039643232,0.000006751365,0.0002526174,0.00030159642,0.00039374287,0.0016687878,0.000057111654,0.00026257135,0.000002874205],"about_ca_topic_score_codex":0.006983903,"about_ca_topic_score_gemma":0.008590036,"teacher_disagreement_score":0.006983903,"about_ca_system_score_codex":0.00048240693,"about_ca_system_score_gemma":0.0001906344,"threshold_uncertainty_score":0.013886511},"labels":[],"label_agreement":null},{"id":"W3009579045","doi":"10.3847/1538-4357/ab7a95","title":"When Gas Dynamics Decouples from Galactic Rotation: Characterizing ISM Circulation in Disk Galaxies","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Comisión Nacional de Investigación Científica y Tecnológica; European Commission; Universität Heidelberg; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Deutsche Forschungsgemeinschaft; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology","keywords":"Physics; Galaxy; Astrophysics; Gravitational potential; Galaxy rotation curve; Interstellar medium; Galactic Center; Rotation (mathematics); Molecular cloud; Astronomy; Galaxy formation and evolution; Stars; Geometry","score_opus":0.013728778532832399,"score_gpt":0.22640889689608634,"score_spread":0.21268011836325396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009579045","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992568,0.00005263473,0.00047783882,0.000019884788,8.1682487e-7,0.0000021836781,0.000037901176,0.000007663257,0.0001442708],"genre_scores_gemma":[0.99984276,0.000012684107,0.00009270652,0.0000018555073,0.0000011057477,9.089884e-7,0.000030964933,0.0000017299536,0.000015263839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999138,0.000028010969,0.000005625257,0.000024873872,0.000009588295,0.0000181169],"domain_scores_gemma":[0.9991916,0.00038021355,0.00017902568,0.000070811395,0.000054323536,0.00012403728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003085601,0.00026198418,0.0002571557,0.00061414053,0.0002449791,0.0007282759,0.000345296,0.00040909083,0.0003280093],"category_scores_gemma":[0.0021994412,0.00017467835,0.00024779927,0.0004252347,0.00073696213,0.0005767849,0.00035316648,0.00020089342,0.000052610267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033763255,0.00015887698,0.6375674,0.000057416444,0.00013273934,0.000353736,0.0003672482,0.32257757,0.028796092,0.0038008522,0.00023836545,0.005612155],"study_design_scores_gemma":[0.00005600283,0.00013381685,0.32801554,0.000012061379,0.000043497697,0.000108323446,0.00020066387,0.6651206,0.003827621,0.002121742,0.00033603865,0.00002413243],"about_ca_topic_score_codex":0.007044661,"about_ca_topic_score_gemma":0.0031298567,"teacher_disagreement_score":0.007044661,"about_ca_system_score_codex":0.0007153047,"about_ca_system_score_gemma":0.00016777028,"threshold_uncertainty_score":0.01400733},"labels":[],"label_agreement":null},{"id":"W3009717748","doi":"10.3847/1538-4357/ab7c5c","title":"The Rarity of Repeating Fast Radio Bursts from Binary Neutron Star Mergers","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Natural Science Foundation of China","keywords":"Magnetar; Neutron star; Millisecond; Binary number; Stars; Star formation; Gravitational wave","score_opus":0.01542018579197828,"score_gpt":0.2883510900261288,"score_spread":0.2729309042341505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009717748","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99825186,0.0003879822,0.00028492868,0.000017548513,0.000003084332,0.0000033555739,0.00012475764,0.000013731283,0.0009127074],"genre_scores_gemma":[0.9995239,0.00009508651,0.00007936573,0.0000045176293,0.000005188109,0.0000011661824,0.00020332065,0.000002254664,0.00008520906],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99976,0.00002367876,0.000018569672,0.00007589715,0.00007764914,0.000044118937],"domain_scores_gemma":[0.9985819,0.00036658146,0.00065786706,0.00012106785,0.00011047643,0.00016223364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028829597,0.00015600765,0.00016624726,0.001110332,0.0002885286,0.0005512231,0.00034189265,0.00027808212,0.0012219661],"category_scores_gemma":[0.0020590217,0.000107093045,0.00016397706,0.0004926792,0.00039925685,0.00021944183,0.00032372214,0.00017246151,0.00020736323],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011980694,0.000007179598,0.9879104,0.000015149646,0.000036024612,0.00034315232,0.000055111843,0.00027961613,0.0041173724,0.0001527076,0.00010047545,0.0068629715],"study_design_scores_gemma":[0.0000030101687,0.000019654412,0.99759114,0.0000039978977,0.000014021721,0.0008727404,0.00003716019,0.00046018726,0.0006724139,0.0000860599,0.00023567969,0.000004091347],"about_ca_topic_score_codex":0.0085140485,"about_ca_topic_score_gemma":0.0064761396,"teacher_disagreement_score":0.0085140485,"about_ca_system_score_codex":0.00035674204,"about_ca_system_score_gemma":0.00016985183,"threshold_uncertainty_score":0.01692897},"labels":[],"label_agreement":null},{"id":"W3009883955","doi":"10.1086/367929","title":"Discovery of A New Class of Pulsating Stars: Gravity-Mode Pulsators among Subdwarf B Stars","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":268,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Stars; Subdwarf; Astrophysics; Astronomy; Opacity; K-type main-sequence star; Light curve; Instability strip; T Tauri star; White dwarf; Cepheid variable","score_opus":0.011171400230312009,"score_gpt":0.23713111687564772,"score_spread":0.2259597166453357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009883955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99855584,0.00021649442,0.000555315,0.000043418047,0.0000043497935,0.000005510823,0.00006392639,0.000020049314,0.0005351144],"genre_scores_gemma":[0.9979159,0.00020760263,0.0011710391,0.00006354236,0.000044624103,0.000009908031,0.00029697572,0.00000594925,0.0002844655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998909,0.000007940749,0.000007711888,0.000044854984,0.000025226671,0.000023225297],"domain_scores_gemma":[0.99919015,0.000120642144,0.0002593363,0.00008817669,0.00007450482,0.000267328],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024833827,0.00020688138,0.00039391077,0.0011847882,0.0007331399,0.00081078784,0.0003418242,0.0005124645,0.0013928794],"category_scores_gemma":[0.0005913819,0.00018914124,0.00015019659,0.0008825449,0.0006071748,0.00058663596,0.0008204557,0.00057632657,0.00035028878],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023068025,0.00009089758,0.9147467,0.000048995455,0.000033813394,0.0005056364,0.00070750876,0.00009588354,0.050058253,0.0006627912,0.00025543474,0.03256338],"study_design_scores_gemma":[0.000017671617,0.0001555063,0.9933687,0.00000771232,0.00001730534,0.001754148,0.0001489145,0.00023424589,0.0017630653,0.00059364847,0.0019302145,0.000008816746],"about_ca_topic_score_codex":0.0005512943,"about_ca_topic_score_gemma":0.00077766494,"teacher_disagreement_score":0.0013928794,"about_ca_system_score_codex":0.00014100646,"about_ca_system_score_gemma":0.00015245329,"threshold_uncertainty_score":0.004659593},"labels":[],"label_agreement":null},{"id":"W3009919203","doi":"10.3847/1538-4357/abce60","title":"Space Telescope and Optical Reverberation Mapping Project. IX. Velocity–Delay Maps for Broad Emission Lines in NGC 5548","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Smithsonian Astrophysical Observatory; University of California, Irvine; Jet Propulsion Laboratory; National Research Foundation of Korea; Nuclear Safety and Security Commission; Science and Technology Facilities Council; National Research Foundation; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; American Academy in Rome; Space Telescope Science Institute; UK Space Agency; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Ohio State University; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Georgia State University; California Institute of Technology; National Aeronautics and Space Administration; Howard Hughes Medical Institute; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; Smithsonian Institution; National Science Foundation","keywords":"Reverberation mapping; Active galactic nucleus; Spectral line; Ellipse; Emission spectrum; Ionization; Telescope; Supermassive black hole; Plane (geometry)","score_opus":0.020922930083532888,"score_gpt":0.26258087322197354,"score_spread":0.24165794313844066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3009919203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8456438,0.00028011497,0.023832774,0.0007113143,0.00015814154,0.00027046612,0.08423021,0.0080523,0.036820892],"genre_scores_gemma":[0.74861723,0.00014226198,0.053030156,0.0001830131,0.00010953054,0.00023522465,0.16034073,0.0011311981,0.036210723],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9998723,0.000015140795,0.0000056169074,0.000030024354,0.000041193114,0.00003564821],"domain_scores_gemma":[0.9995042,0.00003778683,0.000074397845,0.000121296915,0.00013147833,0.00013098524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004613061,0.0003245169,0.00018666753,0.00095575245,0.0003252175,0.00045548455,0.00038651712,0.00021748264,0.009016768],"category_scores_gemma":[0.00068459334,0.00012751175,0.00021926533,0.00058968214,0.00008809056,0.00038296837,0.00041670838,0.00026575403,0.0043412894],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019864286,0.0005703273,0.28474924,0.00012697942,0.00015324386,0.0014423522,0.0020901754,0.00825453,0.12476206,0.0018895724,0.14401957,0.42995548],"study_design_scores_gemma":[0.00021107448,0.00032957376,0.83768016,0.000024638433,0.00005662116,0.00046602,0.00042054508,0.023297833,0.019899175,0.001212371,0.116357714,0.000044257034],"about_ca_topic_score_codex":0.017592091,"about_ca_topic_score_gemma":0.020244006,"teacher_disagreement_score":0.017592091,"about_ca_system_score_codex":0.00035134985,"about_ca_system_score_gemma":0.00027879863,"threshold_uncertainty_score":0.034979403},"labels":[],"label_agreement":null},{"id":"W3010225355","doi":"10.3847/1538-4357/ab9df7","title":"Millimeter-wave Point Sources from the 2500 Square Degree SPT-SZ Survey: Catalog and Population Statistics","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University; Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; Dalhousie University","funders":"","keywords":"Galaxy; Redshift; Source counts; Active galactic nucleus; Population; Point source; Telescope; Millimeter; Flux (metallurgy)","score_opus":0.027505082446714294,"score_gpt":0.21767951127189028,"score_spread":0.190174428825176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3010225355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9245201,0.00024508286,0.0016395425,0.00004779994,0.0000044753933,0.0000808593,0.07047645,0.00026449506,0.0027210817],"genre_scores_gemma":[0.79988015,0.00061773486,0.0024154088,0.000041956682,0.000040996954,0.00021758009,0.19437476,0.00007501089,0.002336346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958533,0.00003945765,0.00006653353,0.000097651166,0.0001537378,0.000057317593],"domain_scores_gemma":[0.99755174,0.00032727333,0.00094783347,0.00034346228,0.00057001703,0.00025971356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000499766,0.0003309904,0.00034295782,0.0058089835,0.0002467294,0.00064045796,0.00047183756,0.00022299543,0.004991275],"category_scores_gemma":[0.001884554,0.00017829034,0.00028408616,0.005459966,0.00019258782,0.0004079986,0.00065441744,0.00020363618,0.003258749],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000065919034,0.000040577394,0.97903377,0.00003887006,0.000054063035,0.00008579084,0.00009400013,0.0006280439,0.0015941891,0.00018287878,0.005584945,0.012597101],"study_design_scores_gemma":[0.000007021031,0.000026941249,0.9961779,0.000006585347,0.00001523123,0.0001560014,0.00005492577,0.00085569685,0.0003227785,0.000049906906,0.0023222286,0.0000048158336],"about_ca_topic_score_codex":0.0048142215,"about_ca_topic_score_gemma":0.003456579,"teacher_disagreement_score":0.0058089835,"about_ca_system_score_codex":0.0002085613,"about_ca_system_score_gemma":0.00025680364,"threshold_uncertainty_score":0.016697466},"labels":[],"label_agreement":null},{"id":"W3010746558","doi":"10.3847/1538-4357/ab7eb4","title":"Reinflation of Warm and Hot Jupiters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Hot Jupiter; Gas giant; Planet; Stars; Light curve; Planetary system; Flux (metallurgy)","score_opus":0.013242897071470448,"score_gpt":0.2146617248108308,"score_spread":0.20141882773936035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3010746558","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987489,0.00007877948,0.0006467634,0.000016390899,0.0000024479018,0.0000030072056,0.000114219496,0.000024222607,0.00036515624],"genre_scores_gemma":[0.9991424,0.000020090194,0.00033914298,0.0000066870334,0.0000017067235,0.0000021266421,0.00017033123,0.000004265172,0.00031334357],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998325,0.00001999758,0.0000067428814,0.00006791474,0.000022069979,0.000050689818],"domain_scores_gemma":[0.9992488,0.00014787074,0.00026636364,0.00011666323,0.000067173256,0.00015306543],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000349324,0.00030479167,0.00029426278,0.00045258863,0.00033460508,0.00054874644,0.0005132024,0.00033037597,0.0018007407],"category_scores_gemma":[0.00094504625,0.00014375016,0.0006784122,0.00021383047,0.00030882613,0.00040033046,0.000527451,0.0002686544,0.00014918418],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071806536,0.00008308394,0.7718507,0.00014202435,0.00039555115,0.0007567347,0.0005684887,0.06697527,0.13779134,0.0026385344,0.00053185946,0.017548429],"study_design_scores_gemma":[0.000020085736,0.00043296182,0.8543823,0.000020792873,0.00010436877,0.0006190481,0.00037835518,0.11692277,0.02349913,0.0015723809,0.002015499,0.000032319855],"about_ca_topic_score_codex":0.0044564386,"about_ca_topic_score_gemma":0.0064040637,"teacher_disagreement_score":0.0044564386,"about_ca_system_score_codex":0.0006169678,"about_ca_system_score_gemma":0.000120445606,"threshold_uncertainty_score":0.008861005},"labels":[],"label_agreement":null},{"id":"W3011042941","doi":"10.1086/512857","title":"Far-Infrared Detection of H <sub>2</sub> D <sup>+</sup> toward Sgr B2","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Mean kinetic temperature; Spectral line; Line (geometry); Infrared; Line-of-sight; Absorption (acoustics); Absorption spectroscopy; Emission spectrum; Far infrared","score_opus":0.009896285202754857,"score_gpt":0.22643025019949964,"score_spread":0.2165339649967448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011042941","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931016,0.00023885416,0.00082583306,0.00006395589,0.000022708471,0.000012560378,0.0005941313,0.00007119509,0.0050691953],"genre_scores_gemma":[0.9951243,0.00007620959,0.0013811096,0.00012327157,0.000037669848,0.00001150022,0.0017033303,0.000014312844,0.0015282889],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.000009712278,0.0000040649447,0.0000360313,0.000036534195,0.000031398984],"domain_scores_gemma":[0.9998324,0.000011463848,0.00003057612,0.00001629183,0.000028061251,0.0000811956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013303547,0.00042474145,0.00016522054,0.00038265943,0.0003330012,0.00039988288,0.00029744132,0.000467396,0.0025466743],"category_scores_gemma":[0.00015678535,0.00016970161,0.0001110035,0.0002305753,0.00021953958,0.00017009105,0.00039417297,0.00026248622,0.00087237963],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007135194,0.00015778159,0.1724209,0.00015333283,0.00007995562,0.0008945263,0.00024006676,0.00023914086,0.8130713,0.00036926652,0.0015801025,0.010079947],"study_design_scores_gemma":[0.00007483038,0.00071789057,0.9284611,0.000016888966,0.000035401004,0.0019075732,0.00025237966,0.0009050199,0.058173582,0.00028183384,0.009147908,0.000025646128],"about_ca_topic_score_codex":0.00082314335,"about_ca_topic_score_gemma":0.0019331318,"teacher_disagreement_score":0.0025466743,"about_ca_system_score_codex":0.00013410521,"about_ca_system_score_gemma":0.000069140624,"threshold_uncertainty_score":0.008519471},"labels":[],"label_agreement":null},{"id":"W3011279855","doi":"10.3847/1538-4357/ab7450","title":"The Structure of Tidal Disruption Event Host Galaxies on Scales of Tens to Thousands of Parsecs","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Physics; Astrophysics; Supermassive black hole; Galaxy; Astronomy; Stellar mass; Galaxy merger; Elliptical galaxy; Star formation","score_opus":0.0075805889208930225,"score_gpt":0.22398916441996697,"score_spread":0.21640857549907394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011279855","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99897885,0.00004994029,0.0001668564,0.000022700639,8.0748134e-7,0.0000024996327,0.0001906267,0.00003135199,0.0005563485],"genre_scores_gemma":[0.99933225,0.00001693338,0.00018053954,0.000007330095,0.000002673892,0.0000024309475,0.00027533353,0.0000047130047,0.00017776681],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998946,0.0000069892035,0.0000047271387,0.000032141077,0.000020970701,0.00004054412],"domain_scores_gemma":[0.9990896,0.00023348704,0.0003278435,0.00006905248,0.00008600377,0.00019405015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016994028,0.00010196367,0.0001334307,0.0012550654,0.00026303134,0.0007091975,0.0003145564,0.00018250351,0.0019147898],"category_scores_gemma":[0.0007266253,0.00014798471,0.00017290906,0.0006468099,0.00031220418,0.0004274994,0.0006831836,0.00020239055,0.00025988027],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006346015,0.000027278415,0.98556733,0.0000100041425,0.00003302433,0.00013426844,0.0002179477,0.0010113446,0.006602243,0.000557895,0.000330481,0.0054446724],"study_design_scores_gemma":[0.0000027300352,0.000012921399,0.99723285,0.0000016519306,0.0000045994784,0.000081995,0.00011005543,0.00188653,0.0003082583,0.00012248367,0.00023286471,0.0000030364245],"about_ca_topic_score_codex":0.00482354,"about_ca_topic_score_gemma":0.0037196085,"teacher_disagreement_score":0.00482354,"about_ca_system_score_codex":0.0003141659,"about_ca_system_score_gemma":0.000102974394,"threshold_uncertainty_score":0.009590924},"labels":[],"label_agreement":null},{"id":"W3011488985","doi":"10.3847/1538-4357/ab8005","title":"A Deep Exposure in High Resolution X-Rays Reveals the Hottest Plasma in the ζ Puppis Wind","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Smithsonian Astrophysical Observatory","keywords":"Plasma; Emission spectrum; Spectral line; Instability; Flux (metallurgy); Shock (circulatory); Line (geometry); Shock wave; Solar wind","score_opus":0.016480614923561013,"score_gpt":0.21828655149331708,"score_spread":0.20180593656975607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011488985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99752,0.00006462449,0.00027587885,0.000036782265,0.00000368794,0.0000035846128,0.00020042418,0.000029878342,0.0018651334],"genre_scores_gemma":[0.9988102,0.0000329339,0.00032569224,0.000027725398,0.000005358058,0.0000025248728,0.00020223638,0.000011762052,0.00058169215],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996185,0.000002778246,0.0000010601367,0.000010744112,0.000008198429,0.000015311089],"domain_scores_gemma":[0.99989176,0.000013613711,0.000019297995,0.000016343995,0.00001115576,0.000047701044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010649434,0.00021405607,0.00020423625,0.0004724176,0.00053978903,0.00039470164,0.00016003168,0.00022865205,0.0023577788],"category_scores_gemma":[0.00016943888,0.00017360621,0.00013687024,0.00017942597,0.00026665677,0.00018378808,0.0005761105,0.00042367086,0.00044235025],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006137354,0.000081857375,0.2958035,0.000059210124,0.00011379879,0.0048762555,0.0014067936,0.000692359,0.6789602,0.0004626259,0.0009027244,0.016026981],"study_design_scores_gemma":[0.0000065474646,0.00006807608,0.9889071,0.000006676716,0.000011319014,0.0007633672,0.00029721594,0.00033036733,0.0076267337,0.00016280747,0.0018150392,0.000004849587],"about_ca_topic_score_codex":0.0013055564,"about_ca_topic_score_gemma":0.0018027732,"teacher_disagreement_score":0.0023577788,"about_ca_system_score_codex":0.00013895257,"about_ca_system_score_gemma":0.00005915329,"threshold_uncertainty_score":0.007887542},"labels":[],"label_agreement":null},{"id":"W3011600565","doi":"10.3847/1538-4357/ab8387","title":"The X-Ray Outburst of the Galactic Center Magnetar over Six Years of Chandra Observations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council","keywords":"Magnetar; Pulsar; Supermassive black hole; Milky Way; Galactic Center; Sagittarius A*","score_opus":0.0216595471209416,"score_gpt":0.28555733450588594,"score_spread":0.26389778738494435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011600565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978817,0.00043979284,0.00011895926,0.00004483748,0.000017033262,0.0000057684992,0.00095684273,0.000028853612,0.00050614536],"genre_scores_gemma":[0.9980405,0.00013001639,0.00015630815,0.000019314966,0.000023783523,0.0000035270432,0.0014351346,0.0000064947963,0.00018503919],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973375,0.000026698373,0.000024951638,0.0000928338,0.00005898411,0.000062755214],"domain_scores_gemma":[0.998928,0.00011195466,0.0004024474,0.000117377946,0.00020279833,0.00023739302],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044428275,0.00027306794,0.00023986882,0.001314543,0.00041899874,0.00075231836,0.00022359345,0.00018242295,0.0005360633],"category_scores_gemma":[0.00084491924,0.00013308368,0.00024242784,0.0007683716,0.00017880465,0.00029369438,0.0007499913,0.00028577747,0.00017650903],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002594874,0.00004673208,0.9788953,0.000047499158,0.00010993656,0.0005582227,0.0003650902,0.00019415238,0.0064293705,0.0000792843,0.0009614646,0.012053455],"study_design_scores_gemma":[0.0000014453317,0.00002594557,0.99822074,0.000007543566,0.00001725128,0.00022193766,0.00009235632,0.00013076789,0.00037338716,0.000010890223,0.00089395384,0.0000038264243],"about_ca_topic_score_codex":0.0065781954,"about_ca_topic_score_gemma":0.012426646,"teacher_disagreement_score":0.0065781954,"about_ca_system_score_codex":0.00037062043,"about_ca_system_score_gemma":0.00019273367,"threshold_uncertainty_score":0.013079822},"labels":[],"label_agreement":null},{"id":"W3011873890","doi":"10.3847/1538-4357/ab7b80","title":"HD 145263: Spectral Observations of Silica Debris Disk Formation via Extreme Space Weathering?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Debris disk; Pyroxene; Space weathering; Olivine; Weathering; Silicate; Interplanetary dust cloud; Photometry (optics); Geology; Astrobiology; Solar System; Physics; Mineralogy; Astrophysics; Geochemistry; Planet; Planetary system; Astronomy; Asteroid; Stars","score_opus":0.02999996750833811,"score_gpt":0.2176146737117462,"score_spread":0.1876147062034081,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3011873890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986771,0.00005780868,0.00009449261,0.000009140332,0.0000031768982,0.0000033742297,0.0003226272,0.0000113763235,0.0008208318],"genre_scores_gemma":[0.99945563,0.000010411456,0.000057460053,0.0000064143114,0.0000025961208,0.0000010697322,0.00033159324,0.0000014472357,0.00013338869],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.0000032425914,0.0000029431194,0.000015995427,0.000014042444,0.000017453418],"domain_scores_gemma":[0.99990535,0.000004211111,0.000036013957,0.0000072176513,0.000012903129,0.00003437679],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000834642,0.00023096034,0.00016715137,0.00039205543,0.00044597493,0.00037148478,0.00016163255,0.00019489284,0.0008971],"category_scores_gemma":[0.00008872867,0.000079792386,0.0001981657,0.00031445743,0.00018225482,0.00012420297,0.0002231481,0.00015598087,0.00024349017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003362878,0.00007904082,0.8915425,0.000029458208,0.000066805536,0.0018428519,0.00032906412,0.0003031543,0.10029281,0.00014942119,0.0005759714,0.0044527217],"study_design_scores_gemma":[0.0000037799036,0.000050818224,0.9954093,0.0000019683291,0.000007323252,0.0006285959,0.00010714947,0.00023178943,0.0027599672,0.000024923846,0.00077062944,0.0000037738128],"about_ca_topic_score_codex":0.007228632,"about_ca_topic_score_gemma":0.010651078,"teacher_disagreement_score":0.007228632,"about_ca_system_score_codex":0.0002987153,"about_ca_system_score_gemma":0.00009711559,"threshold_uncertainty_score":0.014373124},"labels":[],"label_agreement":null},{"id":"W3012660843","doi":"10.3847/1538-4357/ab917d","title":"A Deep CFHT Optical Search for a Counterpart to the Possible Neutron Star–Black Hole Merger GW190814","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Alberta; University of Manitoba; Royal Military College of Canada; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Kilonova; Ejecta; Neutron star; Gravitational wave; Sky; Telescope; Binary number","score_opus":0.019388967706212696,"score_gpt":0.26069497521941004,"score_spread":0.24130600751319733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3012660843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931552,0.00005191281,0.00072276476,0.000095608106,0.0000068845648,0.000015235188,0.00066747126,0.00008501664,0.0051997914],"genre_scores_gemma":[0.99607074,0.0000277746,0.0019155641,0.00004968547,0.000014707517,0.0000064149035,0.0009295814,0.0000119089655,0.00097360235],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999275,0.0000033336248,0.0000020348482,0.0000150205315,0.000020338328,0.000031734635],"domain_scores_gemma":[0.9998344,0.0000146280445,0.000039730774,0.00001626122,0.000027900773,0.000067032546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000117901436,0.00014030635,0.000117851305,0.0008758094,0.00039939428,0.0003250932,0.00018201569,0.00024984684,0.0023688967],"category_scores_gemma":[0.0001762922,0.00012424373,0.00014054698,0.00033107185,0.00012461332,0.00017968554,0.0003802322,0.0002522216,0.00030153085],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055834634,0.00028757122,0.47677082,0.00007873374,0.00012439958,0.004131836,0.00087270787,0.0014832638,0.45667315,0.0008609129,0.004914315,0.05324393],"study_design_scores_gemma":[0.000016204147,0.00014459758,0.97736496,0.000010346442,0.0000340583,0.0011911623,0.0003005756,0.0026108387,0.014201783,0.00015609831,0.003956993,0.000012364071],"about_ca_topic_score_codex":0.007958749,"about_ca_topic_score_gemma":0.021133121,"teacher_disagreement_score":0.007958749,"about_ca_system_score_codex":0.0004215926,"about_ca_system_score_gemma":0.00014297287,"threshold_uncertainty_score":0.015824854},"labels":[],"label_agreement":null},{"id":"W3013215908","doi":"10.3847/1538-4357/ab96cd","title":"Thermally Unstable Cooling Stimulated by Uplift: The Spoiler Clusters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Molecular cloud; Star formation; Radiative cooling; Radio galaxy; Atmospheric pressure; Cooling flow","score_opus":0.008498902894994413,"score_gpt":0.20345393120319316,"score_spread":0.19495502830819875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013215908","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999648,0.000008531173,0.000020358293,0.000004140821,7.727265e-7,0.0000018650852,0.00011654966,0.000009533044,0.00019029286],"genre_scores_gemma":[0.99931204,0.000009342683,0.000072840354,0.00000485278,0.0000024947403,0.0000022708477,0.00040827369,0.000006535481,0.00018135711],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974364,0.00001079554,0.000005898979,0.000060183866,0.000040384963,0.00013909998],"domain_scores_gemma":[0.999302,0.00005989807,0.0002025151,0.00010569094,0.000083434774,0.00024649457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020022622,0.00031063004,0.00036399066,0.0011219227,0.0008044542,0.00068060495,0.00036603812,0.00018494374,0.0009761424],"category_scores_gemma":[0.00049591943,0.0001986282,0.00020853305,0.0006232823,0.00052587624,0.00018755888,0.00069345045,0.00026870667,0.00021480171],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028263016,0.00025983175,0.93061537,0.000042143067,0.00011662471,0.001155958,0.0016085317,0.0031767117,0.04739466,0.00095640187,0.0017736398,0.010073804],"study_design_scores_gemma":[0.000020046598,0.0000705789,0.99571437,0.0000021415854,0.000014305278,0.00012396237,0.00029943686,0.0010494081,0.001950824,0.00006139462,0.0006795266,0.000013850745],"about_ca_topic_score_codex":0.015481153,"about_ca_topic_score_gemma":0.021084147,"teacher_disagreement_score":0.015481153,"about_ca_system_score_codex":0.0005472628,"about_ca_system_score_gemma":0.00035692318,"threshold_uncertainty_score":0.030782044},"labels":[],"label_agreement":null},{"id":"W3013221473","doi":"10.3847/1538-4357/ab8467","title":"The MESAS Project: ALMA Observations of the F-type Stars γ Lep, γ Vir A, and γ Vir B","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Stars; Stellar atmosphere; Wavelength; Atmosphere (unit); Circumstellar dust; Emission spectrum; Spectral line; Circumstellar disk","score_opus":0.029105308764714396,"score_gpt":0.2508664074649595,"score_spread":0.22176109870024507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013221473","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98638076,0.00017096702,0.001070827,0.00013778824,0.000021894088,0.000037664755,0.0054308497,0.0003836145,0.0063655768],"genre_scores_gemma":[0.9854085,0.000080991565,0.005312689,0.00008710141,0.000044538032,0.000028686782,0.0073578362,0.000059658923,0.0016199735],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980134,0.000038524893,0.0000075046823,0.000070402646,0.000054959888,0.000027313237],"domain_scores_gemma":[0.9994344,0.000059314327,0.0001508525,0.00009728379,0.00010566765,0.00015249322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007947463,0.00032246477,0.00021987958,0.0010218001,0.00059456326,0.00067025726,0.00045503583,0.000329774,0.0015558692],"category_scores_gemma":[0.00052347576,0.0001532466,0.00032009406,0.0006048322,0.00020393619,0.00034502716,0.00052916515,0.00031193942,0.00054428435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0034403866,0.0004928492,0.8538516,0.00012494065,0.000531976,0.0007405907,0.0005439989,0.0034614012,0.07465036,0.0014107863,0.013878848,0.046872236],"study_design_scores_gemma":[0.0001658066,0.00014574251,0.98019695,0.00001611684,0.000062736595,0.00017178577,0.00017223935,0.005178655,0.00553761,0.00032829834,0.008009882,0.0000142295185],"about_ca_topic_score_codex":0.007996917,"about_ca_topic_score_gemma":0.018895313,"teacher_disagreement_score":0.007996917,"about_ca_system_score_codex":0.000474341,"about_ca_system_score_gemma":0.00030320225,"threshold_uncertainty_score":0.015900731},"labels":[],"label_agreement":null},{"id":"W3013330073","doi":"10.3847/1538-4357/ab9fa0","title":"IceCube Search for High-energy Neutrino Emission from TeV Pulsar Wind Nebulae","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Nuclear Physics; Ontario Ministry of Research and Innovation; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Office of Science; Helmholtz Alliance for Astroparticle Physics; Chiba University; Pacific Northwest National Laboratory; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; European Regional Development Fund; Bundesministerium für Bildung und Forschung; Battelle; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Fermilab; National Science Foundation; Belgian Federal Science Policy Office; High Energy Physics; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Deutsche Forschungsgemeinschaft; University of Oxford; Fonds De La Recherche Scientifique - FNRS; Ministerio de Ciencia, Innovación y Universidades; Polarforskningssekretariatet; National Research Foundation; Michigan State University; Western Canada Research Grid; Compute Canada; Marquette University; University of Chicago; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy","keywords":"Pulsar; Hadron; Neutrino; Interstellar medium; Neutrino detector","score_opus":0.01400713552888088,"score_gpt":0.2307331692506141,"score_spread":0.2167260337217332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013330073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99203134,0.00011646877,0.0013610848,0.000047299793,0.000008667709,0.000024154222,0.004217252,0.00010938077,0.0020844524],"genre_scores_gemma":[0.97052884,0.00017274274,0.0065854047,0.00007918436,0.00002358342,0.000054934477,0.021663086,0.000048604357,0.000843631],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977285,0.00004452486,0.000011807526,0.00007647363,0.000050717208,0.00004364169],"domain_scores_gemma":[0.9994129,0.00019030637,0.00016070092,0.000068433365,0.00007332592,0.00009444138],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065386074,0.00055072864,0.00043433125,0.0011734483,0.00047357977,0.00082701974,0.00025046433,0.0003028284,0.0014443625],"category_scores_gemma":[0.000687192,0.00021280618,0.00042091834,0.0012432418,0.00019167624,0.00025863593,0.000652931,0.00023220835,0.00036183643],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012668193,0.00022682623,0.9036864,0.000074497,0.0005528724,0.0006176947,0.00016492205,0.007205715,0.05909483,0.000751776,0.0037191021,0.022638569],"study_design_scores_gemma":[0.00009326108,0.0003331206,0.93869025,0.000022241327,0.000222691,0.00056060567,0.00023224959,0.015938725,0.03345969,0.00084214075,0.009584524,0.00002062284],"about_ca_topic_score_codex":0.0031965114,"about_ca_topic_score_gemma":0.0042622825,"teacher_disagreement_score":0.0031965114,"about_ca_system_score_codex":0.00031862894,"about_ca_system_score_gemma":0.00029445867,"threshold_uncertainty_score":0.006355822},"labels":[],"label_agreement":null},{"id":"W3013330379","doi":"10.3847/1538-4357/ab8388","title":"The Planetary Luminosity Problem: “Missing Planets” and the Observational Consequences of Episodic Accretion","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration","keywords":"Planet; Giant planet; Accretion (finance); Gas giant; Population; Stars; Planetary system","score_opus":0.028619906564707125,"score_gpt":0.23640856356018145,"score_spread":0.20778865699547433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013330379","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99022,0.0014173548,0.0023051521,0.0013824477,0.000026181971,0.0000064655164,0.0002958275,0.00003815177,0.004308497],"genre_scores_gemma":[0.99920136,0.00009862913,0.0003361924,0.00009747133,0.00004342201,0.0000020494242,0.00009207803,0.0000054347984,0.00012344726],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9991234,0.00036465446,0.00008493831,0.00019134663,0.00015979925,0.000075865464],"domain_scores_gemma":[0.98557985,0.008136792,0.003808653,0.0012255331,0.0005344104,0.0007147023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002740337,0.00012706449,0.00028084326,0.001424886,0.0008671064,0.0010425498,0.00056131824,0.0008874163,0.0018985405],"category_scores_gemma":[0.019732999,0.0001298326,0.00012595573,0.0011189401,0.0011677442,0.0017535333,0.0011986039,0.00061519595,0.00023041837],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013543923,0.000038526985,0.97800833,0.000070799964,0.000046901227,0.00061981316,0.00067247456,0.00022860177,0.002426552,0.0015494723,0.0007102219,0.01549283],"study_design_scores_gemma":[0.000011805842,0.000043969525,0.9905579,0.00003108859,0.000028076722,0.0018126026,0.00060736627,0.0011258931,0.0008321203,0.002836437,0.0021054521,0.000007171683],"about_ca_topic_score_codex":0.0016542122,"about_ca_topic_score_gemma":0.0020480412,"teacher_disagreement_score":0.002740337,"about_ca_system_score_codex":0.00025028648,"about_ca_system_score_gemma":0.00017400311,"threshold_uncertainty_score":0.014492452},"labels":[],"label_agreement":null},{"id":"W3013339110","doi":"10.3847/1538-4357/ab8310","title":"Evidence for Proton Acceleration up to TeV Energies Based on VERITAS and Fermi-LAT Observations of the Cas A SNR","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Spectral index; Telescope; Supernova remnant; Context (archaeology); Particle acceleration; Proton; Acceleration; Pion; Cutoff; Range (aeronautics)","score_opus":0.08791565857709614,"score_gpt":0.28865768767091143,"score_spread":0.20074202909381528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013339110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99921143,0.00004609323,0.00012478176,0.000009331325,0.0000010533672,9.3975046e-7,0.00009740764,0.000013437005,0.00049546646],"genre_scores_gemma":[0.9995658,0.000017566083,0.00012986152,0.0000050153985,0.0000023268315,0.0000012023567,0.00020118449,0.0000028747088,0.00007413406],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987936,0.000015843063,0.00001111228,0.000036805814,0.000029214814,0.000027711227],"domain_scores_gemma":[0.99924904,0.00020613281,0.0002442252,0.00009667344,0.000091876194,0.00011205965],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037912047,0.00021208465,0.00020522045,0.000958527,0.00027969,0.00059859117,0.00023966699,0.00022565159,0.0011342457],"category_scores_gemma":[0.0008619825,0.00021993283,0.00028733583,0.0003896499,0.00025387085,0.0002506103,0.00051899336,0.00019268278,0.00019606575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092666876,0.000081566024,0.8778108,0.000041042298,0.00015308207,0.00074292143,0.00027729498,0.0010847378,0.10874799,0.0007461048,0.00021753844,0.009170273],"study_design_scores_gemma":[0.00001402876,0.00013071187,0.9925012,0.00000849308,0.000048573154,0.00035966048,0.00007506244,0.001776478,0.004544014,0.00013985726,0.00039400824,0.000008018917],"about_ca_topic_score_codex":0.0029972557,"about_ca_topic_score_gemma":0.0046678735,"teacher_disagreement_score":0.0029972557,"about_ca_system_score_codex":0.0003101802,"about_ca_system_score_gemma":0.00011698369,"threshold_uncertainty_score":0.00595963},"labels":[],"label_agreement":null},{"id":"W3013473929","doi":"10.3847/1538-4357/ab528d","title":"Gravity-dominated Collisions: A Model for the Largest Remnant Masses with Treatment for “Hit and Run” and Density Stratification","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Planetesimal; Smoothed-particle hydrodynamics; Collision; Planet; Merge (version control); Astrophysics; Stratification (seeds); Formation and evolution of the Solar System; Protoplanet; Gravitation; Mechanics; Astronomy; Protoplanetary disk","score_opus":0.02415700470769941,"score_gpt":0.24412254816031886,"score_spread":0.21996554345261946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013473929","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9250771,0.00031939222,0.051003005,0.0011898398,0.00007786111,0.00016265392,0.00093181094,0.00035036282,0.020888025],"genre_scores_gemma":[0.9926139,0.00008720244,0.0023418982,0.000105672654,0.000039419483,0.00006739324,0.00018544783,0.000065340195,0.0044936193],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996377,0.000085551,0.000015954132,0.00007170024,0.000053791926,0.0001353263],"domain_scores_gemma":[0.99853635,0.00039156692,0.00035542957,0.00015024553,0.00014579165,0.00042056703],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012176951,0.0005952161,0.0008699317,0.00092220865,0.001383317,0.0018528715,0.0040672915,0.0019366762,0.0052583553],"category_scores_gemma":[0.003046172,0.000633724,0.0015778863,0.00071430637,0.0018149803,0.0015334731,0.0016155674,0.0012721544,0.00073821296],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018984059,0.00012788347,0.022493877,0.000029365743,0.000073111936,0.00064200937,0.00024121636,0.9191429,0.0011265257,0.053073708,0.0012852156,0.0015743307],"study_design_scores_gemma":[0.000049823477,0.000043284082,0.002736746,0.0000063750813,0.000026684153,0.00007378405,0.000068030764,0.9919418,0.00009753493,0.0044984766,0.00043798084,0.000019358855],"about_ca_topic_score_codex":0.05405839,"about_ca_topic_score_gemma":0.02581192,"teacher_disagreement_score":0.05405839,"about_ca_system_score_codex":0.0020435483,"about_ca_system_score_gemma":0.0014978731,"threshold_uncertainty_score":0.1074875},"labels":[],"label_agreement":null},{"id":"W3013697130","doi":"10.3847/1538-4357/ab8386","title":"Stellar Inclination Angles from Be-star H<i>α</i> Emission Line Profiles","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Stars; Polarization (electrochemistry); Interferometry; Sky; Rotation (mathematics); Stellar rotation; Inclination angle; Linear polarization; Line (geometry)","score_opus":0.019342909920466042,"score_gpt":0.23636708806993398,"score_spread":0.21702417814946795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3013697130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900894,0.0000553662,0.007667335,0.000011612991,0.000003957861,0.000008551254,0.0005353433,0.00018569537,0.0014426466],"genre_scores_gemma":[0.9928945,0.000037424063,0.0054871123,0.000006179439,0.000003457371,0.000004924536,0.0013925262,0.00002957056,0.00014432866],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982184,0.000030987652,0.000011343707,0.000057091907,0.0000541824,0.000024579711],"domain_scores_gemma":[0.9993156,0.00012869466,0.00022721496,0.00010071455,0.00015019251,0.00007753354],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036572854,0.0002637146,0.00023279246,0.0006637138,0.00026892248,0.00043472913,0.0001999477,0.00023833891,0.00072303],"category_scores_gemma":[0.0018617467,0.00016674036,0.0002094395,0.00063573144,0.00011051386,0.00023464311,0.00029679574,0.00023657976,0.0006889783],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032852226,0.00006191889,0.8857909,0.000047579055,0.0000694401,0.000077340395,0.00020532944,0.018631034,0.046125405,0.00033132362,0.0006949105,0.047636315],"study_design_scores_gemma":[0.000014051735,0.000062051164,0.90472084,0.000013711444,0.000034614062,0.00014213692,0.00011998055,0.07418131,0.018498901,0.0003649486,0.001826674,0.000020836136],"about_ca_topic_score_codex":0.0038284718,"about_ca_topic_score_gemma":0.0074291467,"teacher_disagreement_score":0.0038284718,"about_ca_system_score_codex":0.00020139283,"about_ca_system_score_gemma":0.00018187915,"threshold_uncertainty_score":0.0076123476},"labels":[],"label_agreement":null},{"id":"W3014145708","doi":"10.3847/1538-4357/ab86a3","title":"Toward a Full MHD Jet Model of Spinning Black Holes. II. Kinematics and Application to the M87 Jet","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Magnetohydrodynamics; Jet (fluid); Bernoulli's principle; Black hole (networking); Magnetic field; Spinning; Plasma; Rotational symmetry; Kinematics","score_opus":0.01972396101502415,"score_gpt":0.23329749161638857,"score_spread":0.21357353060136441,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3014145708","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6638554,0.0017515804,0.29320887,0.0018191664,0.00026419284,0.00016315293,0.00032413975,0.00037860338,0.038235],"genre_scores_gemma":[0.97963744,0.0005180784,0.014595404,0.00018411623,0.0002249581,0.00007506421,0.00008360715,0.00006651836,0.0046148812],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991465,0.00003232142,0.000004178004,0.000010316527,0.000020965443,0.000017582875],"domain_scores_gemma":[0.9998037,0.000028412178,0.00005270122,0.000024407742,0.000032897467,0.00005784686],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003801343,0.00086196855,0.00067805866,0.00055985147,0.00069218606,0.0012991125,0.0011140539,0.001247511,0.0016256316],"category_scores_gemma":[0.0007719605,0.0004976767,0.0011166326,0.00034088647,0.0012854064,0.00095365354,0.0011811509,0.0006552509,0.0004597045],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000102847895,0.000100134464,0.003969052,0.00007254253,0.000050311126,0.0008080762,0.00023560695,0.8428455,0.007975962,0.13781898,0.0009677306,0.0050532515],"study_design_scores_gemma":[0.000026532092,0.000019004083,0.0005595546,0.0000038663375,0.000004194605,0.00003413452,0.000018709276,0.9863127,0.000089484354,0.012656438,0.00026968104,0.000005832692],"about_ca_topic_score_codex":0.0064131757,"about_ca_topic_score_gemma":0.002047361,"teacher_disagreement_score":0.0064131757,"about_ca_system_score_codex":0.0006913175,"about_ca_system_score_gemma":0.0005595861,"threshold_uncertainty_score":0.012751639},"labels":[],"label_agreement":null},{"id":"W3015251211","doi":"10.3847/1538-4357/ab66c0","title":"Erratum: “QED Phenomena in an Ultrastrong Magnetic Field. II. Electron–Positron Scattering, e<sup>±</sup>–Ion Scattering and Relativistic Bremsstrahlung” (2019, ApJ, 875, 23)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Magnetic confinement fusion research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Bremsstrahlung; Positron; Scattering; Electron; Magnetic field; Electron scattering; Nuclear physics; Ion; Atomic physics; Quantum electrodynamics; Quantum mechanics","score_opus":0.008272326845926386,"score_gpt":0.2401324390868275,"score_spread":0.2318601122409011,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015251211","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0007565732,0.0034037014,0.00041576006,0.05733565,0.8907419,0.000021257243,0.002289514,0.00033957526,0.04469614],"genre_scores_gemma":[0.012159739,0.0063201585,0.00190542,0.06524642,0.105668105,0.00007147046,0.0046399,0.0010145754,0.8029743],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9986091,0.0001438252,0.00019322535,0.00017640983,0.0007626448,0.00011481933],"domain_scores_gemma":[0.9959842,0.00089164986,0.00025664738,0.00027332923,0.0022889255,0.00030529095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017006116,0.0016997926,0.001035837,0.0024232054,0.00484326,0.00403649,0.0018261125,0.0034436793,0.059118014],"category_scores_gemma":[0.009858301,0.00065781723,0.0008344245,0.0019449363,0.0015176703,0.0033574048,0.0014562045,0.005435335,0.040540922],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043071646,0.000007164894,0.00008397803,0.000050732848,0.0000034777465,0.0001560033,0.000026540405,0.000029992703,0.0001107087,0.0019154496,0.9931345,0.00443847],"study_design_scores_gemma":[0.00001797402,0.000018884564,0.0013389311,0.00014235656,0.00001406914,0.00035426748,0.00010674354,0.00016897827,0.00046135797,0.002560548,0.99478865,0.000027179123],"about_ca_topic_score_codex":0.022224085,"about_ca_topic_score_gemma":0.04095826,"teacher_disagreement_score":0.059118014,"about_ca_system_score_codex":0.0043740203,"about_ca_system_score_gemma":0.0032183225,"threshold_uncertainty_score":0.19776946},"labels":[],"label_agreement":null},{"id":"W3015347995","doi":"10.3847/1538-4357/ab66bf","title":"Erratum: “QED Phenomena in an Ultrastrong Magnetic Field. I. Electron–Photon Scattering, Pair Creation, and Annihilation” (2018, ApJ, 869, 44)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Atomic and Subatomic Physics Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Annihilation; Photon; Electron; Scattering; Magnetic field; Nuclear physics; Field (mathematics); Quantum mechanics","score_opus":0.011436080596893895,"score_gpt":0.2644035084221154,"score_spread":0.2529674278252215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015347995","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0007342729,0.002200639,0.000487925,0.04935009,0.9173167,0.000021887015,0.0022563615,0.0004055976,0.027226588],"genre_scores_gemma":[0.017389417,0.008568234,0.003364512,0.071124785,0.17903739,0.00008217722,0.0070815464,0.0017629798,0.71158904],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9983126,0.00018529205,0.00023835346,0.00021139171,0.00092087203,0.0001314702],"domain_scores_gemma":[0.995138,0.0011631965,0.00034940636,0.00037315872,0.0026217913,0.00035450954],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001594596,0.0016698884,0.001014712,0.002563713,0.0044052694,0.003303818,0.001987848,0.0033562004,0.06463773],"category_scores_gemma":[0.014458896,0.000630821,0.00085575227,0.001849798,0.0016991583,0.0038109913,0.0017815713,0.00572544,0.04004589],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003656025,0.000007739971,0.00008276631,0.00006112976,0.0000035885485,0.00018587892,0.000028462671,0.000024209252,0.00009905263,0.0017422893,0.9936393,0.004089106],"study_design_scores_gemma":[0.000022112066,0.00002335856,0.0010513694,0.00021395594,0.00001664522,0.0006279708,0.00012230249,0.00018173587,0.0005847467,0.004062428,0.99306047,0.000032951342],"about_ca_topic_score_codex":0.011007532,"about_ca_topic_score_gemma":0.017059408,"teacher_disagreement_score":0.06463773,"about_ca_system_score_codex":0.003162443,"about_ca_system_score_gemma":0.002816782,"threshold_uncertainty_score":0.21623474},"labels":[],"label_agreement":null},{"id":"W3015601962","doi":"10.3847/1538-4357/ab8ad4","title":"Radiative Transfer Modeling of EC 53: An Episodically Accreting Class I Young Stellar Object","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Protostar; Accretion (finance); Radiative transfer; Luminosity; Young stellar object; Spectral energy distribution; Astronomy; Flux (metallurgy); Brightness; Stars; Star formation; Galaxy","score_opus":0.018986473336202445,"score_gpt":0.24117482165101597,"score_spread":0.22218834831481354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015601962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9907137,0.000041754036,0.006013797,0.00006463797,0.0000052234896,0.000010187205,0.000092756134,0.00009434757,0.0029635336],"genre_scores_gemma":[0.9989209,0.000018796803,0.0005793521,0.00001010168,0.0000026845298,0.0000045694487,0.000038333303,0.000013237341,0.0004119896],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995875,0.000009743936,0.0000014346232,0.0000116672145,0.000006265424,0.000012127658],"domain_scores_gemma":[0.999877,0.00004474964,0.000026964213,0.000011552556,0.000015820755,0.000023856344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017118084,0.00040931356,0.00022312217,0.00020909212,0.00031777922,0.00057835656,0.0005708658,0.00055178243,0.0008463117],"category_scores_gemma":[0.00038195113,0.00017145264,0.0006407092,0.00019148298,0.00032369376,0.00027980385,0.000281016,0.00028960808,0.00015092014],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008338103,0.000068331436,0.01967149,0.0000117496365,0.000027645097,0.00018463905,0.00006175904,0.9673441,0.008660389,0.0011388118,0.0001526216,0.0025950966],"study_design_scores_gemma":[0.000009249821,0.000016503796,0.0037211392,0.0000014595297,0.000006694055,0.000023669698,0.000013976113,0.99530834,0.0006648696,0.00015318133,0.00007715403,0.0000037273667],"about_ca_topic_score_codex":0.020821298,"about_ca_topic_score_gemma":0.0053559397,"teacher_disagreement_score":0.020821298,"about_ca_system_score_codex":0.00085878035,"about_ca_system_score_gemma":0.00031672968,"threshold_uncertainty_score":0.041400194},"labels":[],"label_agreement":null},{"id":"W3015690410","doi":"10.3847/1538-4357/ab88a6","title":"Using the Modified Lognormal Power-law Distribution to Model the Mass Function of NGC 1711","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Log-normal distribution; Power law; Range (aeronautics); Physics; Function (biology); Astrophysics; Limit (mathematics); Distribution (mathematics); Law; Mathematics; Statistics; Statistical physics; Applied mathematics; Mathematical analysis","score_opus":0.03238254365336555,"score_gpt":0.2398198343820484,"score_spread":0.20743729072868286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015690410","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.85621893,0.00025316162,0.13697818,0.0002674328,0.000018861405,0.00005797345,0.0007514955,0.00076180656,0.0046920744],"genre_scores_gemma":[0.9906791,0.000070747235,0.007923224,0.00004037354,0.000009144033,0.00003473705,0.00040275208,0.00008327941,0.00075675675],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998424,0.000052643078,0.000005717238,0.00003782666,0.000034867895,0.000026466616],"domain_scores_gemma":[0.999403,0.00025998196,0.00012670037,0.000077936216,0.00009944911,0.00003294989],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087798684,0.00046988513,0.00020690444,0.0011521763,0.00030264864,0.0006658172,0.0009870826,0.000543558,0.0014820074],"category_scores_gemma":[0.0025449428,0.00014314025,0.0003847413,0.00063067186,0.00041577156,0.0007193787,0.00032235228,0.00037515987,0.0007591441],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011578643,0.000047995458,0.15249577,0.00007223073,0.000089363326,0.00045354947,0.00023599443,0.80033463,0.009333825,0.01187847,0.0018551181,0.02308723],"study_design_scores_gemma":[0.000010035205,0.00002277404,0.037348464,0.000017572236,0.000010554875,0.00016445466,0.000048175876,0.95623523,0.0010851845,0.003987749,0.0010463793,0.000023428676],"about_ca_topic_score_codex":0.024066793,"about_ca_topic_score_gemma":0.0151916435,"teacher_disagreement_score":0.024066793,"about_ca_system_score_codex":0.0012169523,"about_ca_system_score_gemma":0.00030738473,"threshold_uncertainty_score":0.04785347},"labels":[],"label_agreement":null},{"id":"W3015715228","doi":"10.3847/1538-4357/ab781c","title":"Dynamical Equilibrium in the Molecular ISM in 28 Nearby Star-forming Galaxies","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":147,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Galaxy; Astrophysics; Molecular cloud; Star formation; Interstellar medium; Sigma; Stars; Astronomy","score_opus":0.0110506934984709,"score_gpt":0.23576804816360475,"score_spread":0.22471735466513384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3015715228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998901,0.000013097764,0.000024837487,0.0000022324255,1.6856318e-7,6.977847e-7,0.00002174138,0.0000015027698,0.000045599605],"genre_scores_gemma":[0.99987507,0.0000065329987,0.000042163098,0.0000013303195,6.884607e-7,8.172657e-7,0.000052636868,6.4867254e-7,0.000020187234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998703,0.000023101598,0.000008146196,0.00003790008,0.00002509571,0.000035425608],"domain_scores_gemma":[0.99956435,0.00008804616,0.000137646,0.000037060527,0.00004248439,0.00013041959],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025003415,0.00015937869,0.0001881453,0.0008049127,0.000269791,0.0004762977,0.00026155563,0.00022168615,0.00038895648],"category_scores_gemma":[0.0009139438,0.00015488561,0.00013933894,0.0004540217,0.00030335668,0.00025870078,0.00045781664,0.00012107099,0.00010042151],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008211471,0.000028661709,0.9875065,0.0000056193885,0.000036988,0.00008554456,0.0003745057,0.00035972268,0.009647918,0.00006349455,0.000019593963,0.0017894976],"study_design_scores_gemma":[0.0000021763472,0.00003154984,0.9984793,7.4171015e-7,0.000005325437,0.000048851325,0.00011806737,0.0008162062,0.00040671293,0.000024001785,0.00006547161,0.0000016464319],"about_ca_topic_score_codex":0.005821052,"about_ca_topic_score_gemma":0.006244439,"teacher_disagreement_score":0.005821052,"about_ca_system_score_codex":0.00037442025,"about_ca_system_score_gemma":0.000099327415,"threshold_uncertainty_score":0.011574328},"labels":[],"label_agreement":null},{"id":"W3016011246","doi":"10.3847/1538-4357/abb1a8","title":"Simultaneous X-Ray and Radio Observations of the Repeating Fast Radio Burst FRB ∼ 180916.J0158+65","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"","keywords":"Fast radio burst; Astrophysics; X-ray; Astronomy; Physics; Computer science; Optics; Neutron star","score_opus":0.01971082875160574,"score_gpt":0.28113313894273945,"score_spread":0.2614223101911337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016011246","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967487,0.0002152794,0.00015034858,0.000023139572,0.000008938072,0.000012842391,0.0007757242,0.00003356644,0.002031505],"genre_scores_gemma":[0.9958009,0.00011525631,0.0007478006,0.00004548164,0.000013224229,0.000009242465,0.0023881013,0.000014364077,0.0008656441],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983454,0.0000054708994,0.0000061073865,0.00004299963,0.000067137604,0.00004375687],"domain_scores_gemma":[0.99961436,0.000016940761,0.000118642376,0.00003996682,0.0000655093,0.00014451498],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021552219,0.0003153972,0.0003679654,0.0009134076,0.0006089984,0.00056807644,0.00037825908,0.00025714026,0.0014577217],"category_scores_gemma":[0.00036271004,0.00021771977,0.00016318174,0.00075379875,0.00025613655,0.00015934632,0.0005499982,0.00032327833,0.00049548445],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015814864,0.0003252117,0.5538117,0.00017954127,0.00025888186,0.0021270837,0.0010694629,0.0008640966,0.3828368,0.0003141338,0.0021852022,0.054446477],"study_design_scores_gemma":[0.000026643656,0.00009501987,0.9940123,0.000010613802,0.00002540666,0.00041945148,0.0001122657,0.00017371625,0.0021552506,0.000034267658,0.0029230507,0.000012011447],"about_ca_topic_score_codex":0.04087417,"about_ca_topic_score_gemma":0.095878504,"teacher_disagreement_score":0.04087417,"about_ca_system_score_codex":0.0005714382,"about_ca_system_score_gemma":0.00032706815,"threshold_uncertainty_score":0.08127254},"labels":[],"label_agreement":null},{"id":"W3016441562","doi":"10.3847/1538-4357/ab84ea","title":"Erratum: “A Multimass Velocity Dispersion Model of 47 Tucanae Indicates No Evidence for an Intermediate-mass Black Hole” (2019, ApJ, 875, 1)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Velocity dispersion; Dispersion (optics); Astrophysics; Black hole (networking); Galaxy; Optics","score_opus":0.041591089876537694,"score_gpt":0.28288400368153266,"score_spread":0.24129291380499496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016441562","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00456325,0.0010399777,0.0010607563,0.06402682,0.88259786,0.000041107127,0.007509965,0.00072632224,0.038434025],"genre_scores_gemma":[0.0643783,0.0028455737,0.0060832547,0.058341667,0.063477136,0.000105255865,0.01713295,0.0018997014,0.78573614],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9994772,0.000029883568,0.00007886828,0.00009605755,0.0002457561,0.00007216119],"domain_scores_gemma":[0.99649554,0.00050592335,0.00018198318,0.00025014434,0.0022693174,0.00029719117],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008357374,0.0013827822,0.00075985084,0.0020500196,0.0056113135,0.0024545733,0.0021891606,0.0034097915,0.045700997],"category_scores_gemma":[0.008222632,0.0006249901,0.00086257374,0.0013730812,0.0012260952,0.0018551315,0.0012004783,0.004607367,0.021286609],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055991462,0.000011360764,0.0003508064,0.000028666725,0.000006666469,0.00024040659,0.000031375464,0.000140976,0.00013853858,0.00080839056,0.9940806,0.004106186],"study_design_scores_gemma":[0.000052868403,0.000030947787,0.008069308,0.00015035734,0.000053226275,0.00030658537,0.00038668767,0.0010136624,0.0007279077,0.0027959214,0.9863377,0.00007472831],"about_ca_topic_score_codex":0.17538582,"about_ca_topic_score_gemma":0.21173772,"teacher_disagreement_score":0.17538582,"about_ca_system_score_codex":0.0031815066,"about_ca_system_score_gemma":0.0043514273,"threshold_uncertainty_score":0.34872997},"labels":[],"label_agreement":null},{"id":"W3016510643","doi":"10.3847/1538-4357/ab8938","title":"Star Formation Occurs in Dense Gas, but What Does “Dense” Mean?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; IBM (Canada)","funders":"Korea Astronomy and Space Science Institute; National Natural Science Foundation of China; University of Texas at Austin","keywords":"Star formation; Molecular cloud; Millimeter; Galaxy; Luminosity; Line (geometry)","score_opus":0.013749466901526942,"score_gpt":0.2324170615941736,"score_spread":0.21866759469264666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016510643","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945357,0.0017049769,0.0011217918,0.00052539475,0.00001881579,0.000007829313,0.00027531903,0.000015224417,0.001794983],"genre_scores_gemma":[0.99860877,0.000636203,0.00040786478,0.00011607827,0.000038581642,0.0000026744774,0.00009575558,0.0000041941153,0.00008984491],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9994373,0.00014322365,0.00004512409,0.00016643906,0.00010195225,0.00010595797],"domain_scores_gemma":[0.99650794,0.0007088954,0.0015636876,0.00046027589,0.00031926951,0.00043988723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009657094,0.00018450376,0.00041586626,0.0010430008,0.00055769423,0.0017498495,0.0003211324,0.00040414114,0.0013610265],"category_scores_gemma":[0.0037595672,0.00018959444,0.00019950035,0.0013324191,0.0020488757,0.0016907293,0.00094241847,0.00029064482,0.00023444767],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001005449,0.00002835988,0.9794725,0.000097672615,0.00009008945,0.0000996017,0.000847902,0.0002722327,0.0037016724,0.0015068717,0.00037624454,0.013406326],"study_design_scores_gemma":[0.000008750743,0.00007999687,0.98930126,0.000071567636,0.00004536985,0.000592458,0.0018411083,0.00038617404,0.001241644,0.0045140185,0.0019046676,0.000013079831],"about_ca_topic_score_codex":0.003123699,"about_ca_topic_score_gemma":0.004466223,"teacher_disagreement_score":0.003123699,"about_ca_system_score_codex":0.0004186151,"about_ca_system_score_gemma":0.00029211494,"threshold_uncertainty_score":0.0062110424},"labels":[],"label_agreement":null},{"id":"W3016988525","doi":"10.1086/308980","title":"Probing the Magnetic Field with Molecular Ion Spectra","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Magnetic field; Ion; Spectral line; Field (mathematics); Physics; Polyatomic ion; Molecule; Turbulence; Atomic physics; Quantum mechanics","score_opus":0.0042701165942407235,"score_gpt":0.19885908010554995,"score_spread":0.19458896351130922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3016988525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9614676,0.0032235347,0.021924986,0.000234725,0.00006958768,0.000053050204,0.00049921125,0.00057297724,0.011954194],"genre_scores_gemma":[0.9885669,0.00061250135,0.009965919,0.000082134546,0.00004757465,0.000021782134,0.00011956525,0.000025022355,0.0005584861],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997987,0.00003351027,0.000005758427,0.00007537855,0.000048091875,0.000038554084],"domain_scores_gemma":[0.99964666,0.0000934521,0.0001309939,0.000049080525,0.00004357663,0.000036188365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003015639,0.00041022376,0.0002672623,0.0012735667,0.00031158183,0.00062136556,0.00064192124,0.00071214966,0.002337034],"category_scores_gemma":[0.0008657814,0.000270333,0.00018346136,0.0009087434,0.0005958178,0.00075551576,0.00084146723,0.0005593645,0.00059680187],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004152092,0.00006963596,0.015240514,0.0001395139,0.00005310715,0.00022725998,0.00013891487,0.0009368464,0.967139,0.0026655,0.00030583682,0.012668638],"study_design_scores_gemma":[0.0000966846,0.0005884531,0.14260827,0.000075141375,0.0001724076,0.0016228905,0.00029136805,0.021883607,0.8150253,0.007688399,0.009838162,0.000109405555],"about_ca_topic_score_codex":0.00026810452,"about_ca_topic_score_gemma":0.0002542199,"teacher_disagreement_score":0.002337034,"about_ca_system_score_codex":0.00016638079,"about_ca_system_score_gemma":0.00006937396,"threshold_uncertainty_score":0.007818162},"labels":[],"label_agreement":null},{"id":"W3017741047","doi":"10.3847/1538-4357/ab7d3e","title":"A Joint Fermi-GBM and LIGO/Virgo Analysis of Compact Binary Mergers from the First and Second Gravitational-wave Observing Runs","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; Goddard Space Flight Center; Marshall Space Flight Center; Istituto Nazionale di Fisica Nucleare; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Industry Canada; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Russian Foundation for Basic Research; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; ICTP South American Institute for Fundamental Research; Canadian Institute for Advanced Research; Ministero dello Sviluppo Economico; Institut des Origines de Lyon; European Regional Development Fund; Scottish Universities Physics Alliance; Kavli Foundation; National Natural Science Foundation of China; Universities Space Research Association; Science and Engineering Research Board; National Science Foundation; Royal Society; National Aeronautics and Space Administration","keywords":"LIGO; Physics; Gravitational wave; Gamma-ray burst; Astrophysics; Fermi Gamma-ray Space Telescope; Astronomy; Neutron star; Binary number; Sky","score_opus":0.034055624097426705,"score_gpt":0.28818195429516236,"score_spread":0.2541263301977357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3017741047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99875224,0.000038825943,0.0002973295,0.00001368484,0.000001111764,0.000003293288,0.00045053617,0.000046603218,0.00039645858],"genre_scores_gemma":[0.99689204,0.000015928576,0.0005818688,0.0000065014497,0.000003679897,0.000003801006,0.0022235552,0.000016173815,0.0002564141],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971944,0.000043157404,0.000014768138,0.000062701074,0.00007179156,0.00008821238],"domain_scores_gemma":[0.999303,0.00018949044,0.00020585007,0.00009893932,0.00007685089,0.00012587778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003930567,0.00032972023,0.00033476655,0.0021459372,0.00029122506,0.0008639441,0.00028300105,0.00026592994,0.0009780215],"category_scores_gemma":[0.0012712423,0.00015805432,0.00061065867,0.0012085319,0.0002185315,0.00029519288,0.00070046005,0.00021675993,0.00026085635],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012287545,0.00012003865,0.9422115,0.000037124868,0.00033353773,0.0006462863,0.00022548369,0.015600906,0.01844394,0.0007683283,0.00079393276,0.019590117],"study_design_scores_gemma":[0.00002220192,0.00010100755,0.9637126,0.000007819381,0.000111648005,0.00033003357,0.00016924586,0.030988414,0.0035430824,0.00017284897,0.0008220534,0.000019038254],"about_ca_topic_score_codex":0.012084874,"about_ca_topic_score_gemma":0.016422492,"teacher_disagreement_score":0.012084874,"about_ca_system_score_codex":0.00038817397,"about_ca_system_score_gemma":0.00034204373,"threshold_uncertainty_score":0.024029076},"labels":[],"label_agreement":null},{"id":"W3018097584","doi":"10.3847/1538-4357/ab7915","title":"Atacama Cosmology Telescope: Dusty Star-forming Galaxies and Active Galactic Nuclei in the Equatorial Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"D-Wave Systems (Canada); University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Active galactic nucleus; Galaxy; Flux (metallurgy); Cosmology; Black-body radiation; Spectral line; Quasar; Telescope; Milky Way","score_opus":0.020474775228327937,"score_gpt":0.24003587523270603,"score_spread":0.2195611000043781,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3018097584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9455907,0.00092623115,0.002107393,0.00012056538,0.000029705472,0.00009675059,0.036460873,0.000268905,0.014398967],"genre_scores_gemma":[0.921117,0.00065355323,0.005592333,0.00014349622,0.0001207158,0.00008456731,0.067511894,0.0000699122,0.004706516],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981076,0.000024292522,0.000016875825,0.000053734577,0.00006535866,0.000028990504],"domain_scores_gemma":[0.99930537,0.000049056798,0.00019621332,0.00011555035,0.0001736238,0.00016019584],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042513866,0.00022442707,0.000247955,0.0022001422,0.00039156032,0.00051419117,0.00035106423,0.00012839829,0.005045311],"category_scores_gemma":[0.0005326764,0.000120568206,0.00015134455,0.0023799988,0.0001303203,0.00023485396,0.0004716464,0.00013847549,0.0011525028],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010119631,0.000043527558,0.9641443,0.00004869916,0.00004399363,0.00007657625,0.00015217261,0.00022721187,0.005182029,0.0002652832,0.0063811815,0.02333382],"study_design_scores_gemma":[0.000005456266,0.0000068626964,0.99527717,0.0000040820514,0.000007935475,0.00004991616,0.000032483946,0.00020392759,0.00028115636,0.000027051246,0.0041022925,0.0000015202799],"about_ca_topic_score_codex":0.02055335,"about_ca_topic_score_gemma":0.025673635,"teacher_disagreement_score":0.02055335,"about_ca_system_score_codex":0.00032358238,"about_ca_system_score_gemma":0.00035233193,"threshold_uncertainty_score":0.040867448},"labels":[],"label_agreement":null},{"id":"W3018109274","doi":"10.3847/1538-4357/ab7af9","title":"A Search for Neutrino Point-source Populations in 7 yr of IceCube Data with Neutrino-count Statistics","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Chiba University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; National Research Foundation; Michigan State University; University of Oxford; Compute Canada; Marquette University","keywords":"Neutrino; Population; Poisson distribution; Milky Way; Context (archaeology); Fermi Gamma-ray Space Telescope; Data set; Neutrino detector","score_opus":0.04381122591996907,"score_gpt":0.28517804499294347,"score_spread":0.24136681907297441,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3018109274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9754532,0.00018180082,0.02007597,0.00013327014,0.000009834631,0.000031085878,0.0020795926,0.00014744457,0.0018876839],"genre_scores_gemma":[0.9805927,0.00006332908,0.012522094,0.000039878807,0.000017465796,0.00003472498,0.0064877216,0.000056874305,0.00018516359],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99799156,0.00096683815,0.00009035374,0.000382884,0.00041589,0.00015245586],"domain_scores_gemma":[0.98790157,0.009146185,0.0011773981,0.0009699631,0.000542372,0.00026255898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005180072,0.0003233628,0.00060869375,0.0016208584,0.00055984856,0.001428664,0.0008563665,0.0006925064,0.0011367351],"category_scores_gemma":[0.011773231,0.00028975584,0.0009757748,0.0015150013,0.0006531613,0.00076588907,0.00087168074,0.0007032684,0.00019150124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084729545,0.00016854724,0.82492024,0.000121547506,0.0009431531,0.0006128006,0.00038550983,0.11607703,0.019940577,0.0107906815,0.0023183683,0.022874327],"study_design_scores_gemma":[0.000089864094,0.00019233012,0.46463922,0.00005286093,0.00020108158,0.0008384155,0.0003076359,0.5022311,0.016334526,0.009239903,0.0058099334,0.00006302026],"about_ca_topic_score_codex":0.0043221493,"about_ca_topic_score_gemma":0.0063932566,"teacher_disagreement_score":0.005180072,"about_ca_system_score_codex":0.00071513874,"about_ca_system_score_gemma":0.000730011,"threshold_uncertainty_score":0.027395189},"labels":[],"label_agreement":null},{"id":"W3018604819","doi":"10.3847/1538-4357/ab8d25","title":"WISEA J083011.95+283716.0: A Missing Link Planetary-mass Object","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Parallax; Brown dwarf; Planet; Object (grammar); Population; Flux (metallurgy)","score_opus":0.016322684894218887,"score_gpt":0.22180366917445873,"score_spread":0.20548098428023984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3018604819","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98736644,0.00020983334,0.0010484905,0.0003390629,0.00006152813,0.000023597742,0.0018343786,0.00030404812,0.008812508],"genre_scores_gemma":[0.99147356,0.00007627605,0.0015834356,0.00020959107,0.00003924965,0.000018132601,0.0038712812,0.0000398062,0.0026886207],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988246,0.0000044678773,0.0000065433733,0.000028122937,0.00003884094,0.00003954979],"domain_scores_gemma":[0.99956495,0.000023352048,0.000105249266,0.00006522859,0.000059302503,0.00018188893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017826959,0.0002046214,0.0003564894,0.00095536414,0.00091234985,0.00063170417,0.0003380097,0.00043814606,0.003994719],"category_scores_gemma":[0.00036920735,0.00013987007,0.00023803461,0.0006185401,0.00027819854,0.00032658616,0.00092303986,0.00034824118,0.002082182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007700746,0.00036493628,0.7408259,0.00024303253,0.00009818363,0.008332283,0.0015282077,0.00034708314,0.13141818,0.0028806727,0.029229334,0.083962195],"study_design_scores_gemma":[0.00003789017,0.00022351931,0.9357434,0.000047818525,0.00005750231,0.005251357,0.0010491791,0.0012175004,0.010003979,0.0008142343,0.045526635,0.00002703788],"about_ca_topic_score_codex":0.0024428475,"about_ca_topic_score_gemma":0.0048427754,"teacher_disagreement_score":0.003994719,"about_ca_system_score_codex":0.00028852888,"about_ca_system_score_gemma":0.00023970995,"threshold_uncertainty_score":0.013363719},"labels":[],"label_agreement":null},{"id":"W3018740860","doi":"10.3847/1538-4357/ab7f29","title":"Planes of Satellites around Simulated Disk Galaxies. I. Finding High-quality Planar Configurations from Positional Information and Their Comparison to MW/M31 Data","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leibniz-Gemeinschaft; Universidad Andrés Bello; Universidad de Chile; Ministerio de Ciencia e Innovación; European Commission","keywords":"Planar; Galaxy; Physics; Satellite; Zoom; Astrophysics; Kinematics; Plane (geometry); Satellite galaxy; Quality (philosophy); Computer science; Reference frame; Galaxy formation and evolution; Frame (networking); Geometry; Astronomy; Computer graphics (images); Optics; Mathematics","score_opus":0.03057457799238223,"score_gpt":0.2622505012665371,"score_spread":0.23167592327415487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3018740860","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99513227,0.00011427365,0.0027810188,0.000029097971,0.0000047118892,0.000015413547,0.0010963932,0.00013312479,0.00069356523],"genre_scores_gemma":[0.995037,0.000042635496,0.0032572576,0.000006369933,0.0000034375666,0.0000074722193,0.0015299048,0.000035313486,0.0000805137],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982387,0.00004104751,0.000012429692,0.000044298922,0.000041472675,0.000036969388],"domain_scores_gemma":[0.9985721,0.00045241896,0.00037134864,0.00023990823,0.00018181608,0.00018233476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044622814,0.00037577606,0.0003353022,0.0012766868,0.00029311955,0.00059905776,0.0005928987,0.00048156595,0.0009894298],"category_scores_gemma":[0.0027220596,0.00030372883,0.0004290567,0.0010067602,0.00046241886,0.00041709666,0.00050722377,0.0002974785,0.0001676096],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050055794,0.00012576544,0.2119657,0.00014021361,0.00021114502,0.00039371874,0.00038989162,0.76245266,0.011080001,0.0022414674,0.0008052981,0.009693649],"study_design_scores_gemma":[0.00005967338,0.00010674526,0.07905076,0.00003594826,0.00004119869,0.00014858902,0.00029315794,0.91376466,0.004214688,0.0012365432,0.0010078617,0.00004015584],"about_ca_topic_score_codex":0.009625913,"about_ca_topic_score_gemma":0.0077173463,"teacher_disagreement_score":0.009625913,"about_ca_system_score_codex":0.00050291524,"about_ca_system_score_gemma":0.00032802744,"threshold_uncertainty_score":0.019139767},"labels":[],"label_agreement":null},{"id":"W3019205829","doi":"10.3847/1538-4357/ab8d3e","title":"ALMA ACA and Nobeyama Observations of Two Orion Cores in Deuterated Molecular Lines","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"IBM (Canada); University of Victoria; McMaster University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Outflow; Molecular cloud; Line (geometry); Submillimeter Array; Stars; Core (optical fiber); Star formation; Emission spectrum","score_opus":0.024614920997056946,"score_gpt":0.2609032556515203,"score_spread":0.23628833465446333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3019205829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938464,0.000018648137,0.000057741556,0.0000063734847,0.0000015202111,0.0000030930755,0.000062887484,0.0000055236505,0.00045952047],"genre_scores_gemma":[0.99908686,0.000012273744,0.00032788294,0.00001235758,0.000004825187,0.00000608032,0.00030087255,0.0000039319057,0.0002448436],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998783,0.000008208391,0.0000038076435,0.00003777358,0.000037112848,0.0000347887],"domain_scores_gemma":[0.9996289,0.000025171954,0.000066438784,0.000037542675,0.00007675845,0.00016512808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013413359,0.000168908,0.00019412096,0.00068262056,0.0003920231,0.00033501204,0.00030652585,0.000245373,0.00060101907],"category_scores_gemma":[0.0002960748,0.00019146928,0.00018184239,0.00032551464,0.00016156012,0.00019167367,0.00063964666,0.00018951925,0.00013647835],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005759583,0.00014343752,0.79482067,0.000026941985,0.00009461636,0.0007272627,0.0010157226,0.00027459973,0.19179995,0.00022322201,0.00033738304,0.00996026],"study_design_scores_gemma":[0.000010296179,0.00003283407,0.99671566,0.000002374272,0.000012108217,0.000058516594,0.00012722971,0.00045590027,0.0020594904,0.000016595424,0.00050633244,0.0000027346346],"about_ca_topic_score_codex":0.00845078,"about_ca_topic_score_gemma":0.019263474,"teacher_disagreement_score":0.00845078,"about_ca_system_score_codex":0.00037275246,"about_ca_system_score_gemma":0.00015986741,"threshold_uncertainty_score":0.016803145},"labels":[],"label_agreement":null},{"id":"W3020936581","doi":"10.3847/1538-4357/ab910e","title":"VERITAS Discovery of VHE Emission from the Radio Galaxy 3C 264: A Multiwavelength Study","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Crab Nebula; Radio galaxy; Flux (metallurgy); Spectral index; Galaxy; Spectral energy distribution; Quasar; Active galactic nucleus; X-shaped radio galaxy","score_opus":0.012838225216533416,"score_gpt":0.22490104022198656,"score_spread":0.21206281500545315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3020936581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99852824,0.000159608,0.00018097671,0.000033499364,0.000006448909,0.000008351998,0.0003656179,0.000019535999,0.00069760997],"genre_scores_gemma":[0.9970613,0.0001160943,0.0006241187,0.00003784349,0.00003258826,0.000004859962,0.001627771,0.000013310219,0.00048208243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986076,0.0000070744672,0.000005291472,0.000037456317,0.000048260266,0.000041156945],"domain_scores_gemma":[0.9995932,0.00003068046,0.000121061894,0.000043710817,0.000060705213,0.00015074256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025755443,0.0002101394,0.0001959542,0.0016151182,0.00045275583,0.00052288454,0.00028110816,0.0002071277,0.0007059019],"category_scores_gemma":[0.00022354699,0.00017821064,0.00027026908,0.00072264666,0.00032724967,0.0001974469,0.00069360016,0.00040124648,0.00022317111],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040647076,0.00025261004,0.8502494,0.00006463317,0.000119428696,0.0029790022,0.0005698619,0.00042459607,0.124120586,0.00039508034,0.0012286435,0.019189712],"study_design_scores_gemma":[0.000007152593,0.00007314503,0.99595153,0.0000069129756,0.000018714942,0.0005109164,0.00013837875,0.00031813717,0.0014720443,0.00004364741,0.0014516347,0.000007721054],"about_ca_topic_score_codex":0.007070846,"about_ca_topic_score_gemma":0.011902364,"teacher_disagreement_score":0.007070846,"about_ca_system_score_codex":0.00037698544,"about_ca_system_score_gemma":0.00022271197,"threshold_uncertainty_score":0.014059365},"labels":[],"label_agreement":null},{"id":"W3021154744","doi":"10.3847/1538-4357/ab8f9a","title":"Orphan GRB Afterglow Searches with the Pan-STARRS1 COSMOS Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Saint Mary's University","funders":"","keywords":"Gamma-ray burst; Afterglow; Galaxy; Jet (fluid); Cosmos (plant); Limiting magnitude","score_opus":0.02563753781412324,"score_gpt":0.23416308245169437,"score_spread":0.20852554463757114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3021154744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956316,0.00008326939,0.00049307384,0.00004275481,0.000003603234,0.000021484942,0.0025119283,0.000074030824,0.0011383606],"genre_scores_gemma":[0.9878648,0.00013476031,0.0018069429,0.000016993235,0.000014452096,0.00002134908,0.009443658,0.00002156992,0.00067548256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965465,0.00009228247,0.000021985372,0.00009145585,0.000079670215,0.000059967682],"domain_scores_gemma":[0.9989071,0.00014815989,0.00027619,0.00019175016,0.00017972918,0.00029714257],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009055458,0.00030592558,0.00029511857,0.002159856,0.00024630516,0.00044134253,0.00023019573,0.00015173237,0.0020241828],"category_scores_gemma":[0.0011168406,0.00010955882,0.00024931334,0.0013963645,0.00014418451,0.00026002104,0.000856933,0.0001570126,0.0005148525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003156556,0.00003688817,0.96837956,0.000048530444,0.00007962785,0.0002491492,0.00014582125,0.0009218582,0.0053569004,0.00022725567,0.0016078252,0.022631034],"study_design_scores_gemma":[0.000012766451,0.00007075141,0.99498993,0.000006349399,0.000031905245,0.00020780029,0.00013407003,0.0014289637,0.0010265933,0.00007355903,0.002011834,0.0000054876878],"about_ca_topic_score_codex":0.004193796,"about_ca_topic_score_gemma":0.0061596325,"teacher_disagreement_score":0.004193796,"about_ca_system_score_codex":0.00021716786,"about_ca_system_score_gemma":0.0003069557,"threshold_uncertainty_score":0.008338749},"labels":[],"label_agreement":null},{"id":"W3021237625","doi":"10.1088/0004-637x/733/2/109","title":"DISPERSION OF MAGNETIC FIELDS IN MOLECULAR CLOUDS. III.","year":2011,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Ambipolar diffusion; Lambda; Molecular cloud; Astrophysics; Magnetic field; Polarization (electrochemistry); Spectral density; Stars; Optics","score_opus":0.00932475027414814,"score_gpt":0.21411446670248915,"score_spread":0.204789716428341,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3021237625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92961866,0.0006892511,0.063546084,0.00018904735,0.000049074795,0.00003094288,0.00031760597,0.00042733623,0.0051320274],"genre_scores_gemma":[0.9844726,0.00023505985,0.014569214,0.000025781075,0.000039503982,0.000013656181,0.00012894486,0.000021316551,0.0004938626],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999026,0.000008841708,0.0000048787315,0.000022035016,0.0000385834,0.000023042123],"domain_scores_gemma":[0.99972206,0.00008218705,0.00006985136,0.00007272389,0.000037119506,0.00001606071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002369938,0.00017163847,0.00014521588,0.001321072,0.00035779004,0.00048100392,0.0002427894,0.00024465955,0.00062258524],"category_scores_gemma":[0.0012853189,0.000111067246,0.00024867945,0.0008276819,0.00032313014,0.0002815054,0.00038724442,0.00040755214,0.00028836055],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022033796,0.00011016755,0.31175438,0.00021538022,0.00020504407,0.0008579747,0.0010358581,0.039560992,0.39730552,0.027553309,0.0012515847,0.21992944],"study_design_scores_gemma":[0.000054528577,0.00016695882,0.60956997,0.00007423422,0.00007424094,0.002176548,0.0004955789,0.21694565,0.13547051,0.02476832,0.0101148235,0.00008866271],"about_ca_topic_score_codex":0.004329857,"about_ca_topic_score_gemma":0.0030022257,"teacher_disagreement_score":0.004329857,"about_ca_system_score_codex":0.00032604512,"about_ca_system_score_gemma":0.00010920013,"threshold_uncertainty_score":0.008609295},"labels":[],"label_agreement":null},{"id":"W3022063716","doi":"10.3847/1538-4357/ab9110","title":"Magnetic Field Structure in Spheroidal Star-forming Clouds. II. Estimating Field Structure from Observed Maps","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Field strength; Magnetic field; Polarization (electrochemistry); Envelope (radar); Field (mathematics); Resolution (logic); Flux (metallurgy)","score_opus":0.01317598538360277,"score_gpt":0.22256196405521672,"score_spread":0.20938597867161396,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3022063716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97622013,0.00027287946,0.021307215,0.00004192324,0.0000040272894,0.000023976996,0.00045971823,0.00022615492,0.0014440232],"genre_scores_gemma":[0.9964386,0.000061447834,0.003154475,0.000002800362,0.0000044292888,0.000004762513,0.0002209498,0.000008514536,0.00010401526],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999517,0.000008472129,0.0000016191652,0.0000118079715,0.000015325075,0.000010972723],"domain_scores_gemma":[0.9998149,0.000044930603,0.000052390013,0.000028415314,0.000034557812,0.000024762518],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015884767,0.00024159855,0.00017843643,0.0007863629,0.00022668538,0.0004706494,0.0003811378,0.00018786457,0.00033240646],"category_scores_gemma":[0.0008742328,0.00019514964,0.00020586603,0.0004176638,0.00021271771,0.0004210592,0.00020670096,0.00014448976,0.00014036054],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020236878,0.000049282095,0.49552384,0.00008524989,0.00008990035,0.00018098886,0.00021057238,0.42114753,0.037660126,0.003340821,0.000642132,0.040867146],"study_design_scores_gemma":[0.000015352487,0.00002828865,0.24402675,0.000013494375,0.000012975794,0.00010921416,0.00008349404,0.7473638,0.0053992593,0.002201566,0.00072890904,0.000016887108],"about_ca_topic_score_codex":0.016333546,"about_ca_topic_score_gemma":0.010502041,"teacher_disagreement_score":0.016333546,"about_ca_system_score_codex":0.0007218441,"about_ca_system_score_gemma":0.00022065979,"threshold_uncertainty_score":0.03247696},"labels":[],"label_agreement":null},{"id":"W3022133077","doi":"10.3847/1538-4357/abb1c0","title":"Star Formation and Morphological Properties of Galaxies in the Pan-STARRS 3π Survey. I. A Machine-learning Approach to Galaxy and Supernova Classification","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Heising-Simons Foundation","keywords":"Galaxy; Supernova; Random forest; Star formation; Observatory; Stars; Galaxy formation and evolution","score_opus":0.047110621351856626,"score_gpt":0.2290727758381194,"score_spread":0.1819621544862628,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3022133077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9885711,0.00037644125,0.004683549,0.00019753863,0.000010069239,0.000036585534,0.004737497,0.0005411255,0.0008461245],"genre_scores_gemma":[0.98099893,0.0001200294,0.006359146,0.000042437343,0.000026038935,0.000024582549,0.01203984,0.000043352084,0.00034565898],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995635,0.00012020594,0.00003314455,0.00011318481,0.00012124431,0.000048646765],"domain_scores_gemma":[0.9988469,0.00040168295,0.0002400841,0.00025360403,0.00014808415,0.00010958996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001387855,0.00045719388,0.0003634631,0.0019267383,0.00022415227,0.0006352415,0.00056818285,0.0005181022,0.0007488018],"category_scores_gemma":[0.0027962613,0.00015568665,0.0006990663,0.0009306388,0.00028028176,0.0005345777,0.00045685997,0.00059847994,0.00065718434],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003476821,0.00018326225,0.8655963,0.000116710085,0.00017466705,0.000060365965,0.00008512325,0.048878968,0.0071562664,0.0004799885,0.0040059644,0.072914824],"study_design_scores_gemma":[0.00006063109,0.0002050218,0.7674635,0.000034513727,0.000050624454,0.00014291386,0.000107886925,0.22168319,0.0067441845,0.0008671724,0.0026139296,0.000026425267],"about_ca_topic_score_codex":0.0119038,"about_ca_topic_score_gemma":0.014334321,"teacher_disagreement_score":0.0119038,"about_ca_system_score_codex":0.00052004616,"about_ca_system_score_gemma":0.000286413,"threshold_uncertainty_score":0.023669004},"labels":[],"label_agreement":null},{"id":"W3022292055","doi":"10.3847/1538-4357/aba94f","title":"Gamma-Ray Urgent Archiver for Novel Opportunities (GUANO): Swift/BAT Event Data Dumps on Demand to Enable Sensitive Subthreshold GRB Searches","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Gamma-ray burst; Observatory; Event (particle physics); Pipeline (software); Telescope; Automation","score_opus":0.11219158422732434,"score_gpt":0.28578198291190154,"score_spread":0.1735903986845772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3022292055","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5493125,0.0011639699,0.09290663,0.0022332391,0.001190873,0.0015707549,0.089366265,0.2040823,0.058173604],"genre_scores_gemma":[0.8161475,0.00027816507,0.094676875,0.00078055257,0.0003394681,0.00072407565,0.075391084,0.004650467,0.007011821],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993755,0.000069200214,0.000045499226,0.00017185498,0.00023956534,0.000098328106],"domain_scores_gemma":[0.99731594,0.00026150548,0.0003280821,0.0012187322,0.0004339587,0.00044168232],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001239345,0.00056384515,0.00042841464,0.0013927434,0.00048107776,0.0012444373,0.0009112708,0.00038247657,0.0046073827],"category_scores_gemma":[0.0028849288,0.00035500128,0.00026183485,0.0008690829,0.00034395192,0.0009367491,0.0021444682,0.00090179854,0.0027268676],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0049660546,0.00068783865,0.22502862,0.000504226,0.000353885,0.002264161,0.0021113108,0.01377784,0.12573285,0.008411725,0.2733955,0.342766],"study_design_scores_gemma":[0.0012969027,0.00078267534,0.17571828,0.00024481147,0.00015725213,0.00086037896,0.000950035,0.22660214,0.12166374,0.00870212,0.46263608,0.00038567968],"about_ca_topic_score_codex":0.0058772643,"about_ca_topic_score_gemma":0.007957842,"teacher_disagreement_score":0.0058772643,"about_ca_system_score_codex":0.000474604,"about_ca_system_score_gemma":0.00093432714,"threshold_uncertainty_score":0.015413225},"labels":[],"label_agreement":null},{"id":"W3022315906","doi":"10.3847/1538-4357/ababa9","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Mg ii Lag Results from Four Years of Monitoring","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Lag; Quasar; Sky; Reverberation mapping; Supermassive black hole; Redshift; Reverberation; Accretion (finance)","score_opus":0.02665796927796833,"score_gpt":0.22651528729339004,"score_spread":0.19985731801542173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3022315906","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99181646,0.0001424127,0.00037226628,0.000051603107,0.000011220677,0.000015124105,0.006350264,0.0000698523,0.0011708009],"genre_scores_gemma":[0.9769325,0.00007185382,0.0006231755,0.000038280978,0.000025543077,0.000025275027,0.021577155,0.000037651887,0.00066861336],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988285,0.00016622762,0.00011608133,0.00026502495,0.0003856484,0.00023856443],"domain_scores_gemma":[0.99382836,0.0006530585,0.002519832,0.0010067429,0.0012650759,0.0007269709],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002008204,0.00037158304,0.00027799598,0.002199116,0.0003436117,0.0007886017,0.00045422695,0.00029576558,0.0008732171],"category_scores_gemma":[0.0039582937,0.00015694315,0.0003711039,0.0014788489,0.0002884906,0.00054291904,0.0010421522,0.00027734446,0.00060321845],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014205373,0.000029563666,0.9898865,0.000021836022,0.000078124736,0.00007435701,0.00022728152,0.00040365773,0.00085101026,0.000043955522,0.001702605,0.0065390067],"study_design_scores_gemma":[0.0000034956688,0.0000205369,0.99834204,0.0000033452939,0.000014472268,0.00003421676,0.00006881294,0.00020576981,0.00041183352,0.000010184134,0.0008817762,0.0000035633977],"about_ca_topic_score_codex":0.02533831,"about_ca_topic_score_gemma":0.041700028,"teacher_disagreement_score":0.02533831,"about_ca_system_score_codex":0.00058026146,"about_ca_system_score_gemma":0.00029450137,"threshold_uncertainty_score":0.05038166},"labels":[],"label_agreement":null},{"id":"W3022494508","doi":"10.3847/1538-4357/ab845c","title":"Spectroscopic Constraints on the Buildup of Intracluster Light in the Coma Cluster","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Coma Cluster; Galaxy; Stellar population; Metallicity; Astronomy; Velocity dispersion; Surface brightness; Intracluster medium; Population; Galaxy cluster; Stars; Star formation; Medicine","score_opus":0.009424933982488271,"score_gpt":0.21438941446584842,"score_spread":0.20496448048336013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3022494508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99949634,0.000012501192,0.000053163392,0.0000033183546,2.7674466e-7,7.562493e-7,0.00006668247,0.0000060745456,0.00036091718],"genre_scores_gemma":[0.9998598,0.0000045696756,0.000034968372,0.0000013403941,7.3765324e-7,5.7709315e-7,0.00006963649,0.0000012011778,0.000027005904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998946,0.0000093469,0.000004546513,0.000024817002,0.000027079133,0.000039594837],"domain_scores_gemma":[0.9993974,0.000084015905,0.00018725781,0.000060979466,0.00011117621,0.00015920018],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000113386835,0.00023101232,0.00017123144,0.0008229037,0.00042804153,0.00037249317,0.00021641298,0.00012430025,0.0013787926],"category_scores_gemma":[0.0006479563,0.000114237686,0.00009229748,0.0004203279,0.0002871496,0.00017460393,0.0003782066,0.000094554176,0.00027410948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001119767,0.000017306453,0.97369385,0.000005683051,0.000016474167,0.000060532606,0.00011579428,0.0003332723,0.022957755,0.00012216302,0.00008418062,0.0024810121],"study_design_scores_gemma":[0.000001993523,0.000015549273,0.99805486,0.0000015198659,0.0000056658782,0.00003602009,0.00008112409,0.00057709153,0.0010758456,0.00003224488,0.00011632642,0.0000016816421],"about_ca_topic_score_codex":0.008835935,"about_ca_topic_score_gemma":0.012670137,"teacher_disagreement_score":0.008835935,"about_ca_system_score_codex":0.00035056926,"about_ca_system_score_gemma":0.00009255113,"threshold_uncertainty_score":0.017569005},"labels":[],"label_agreement":null},{"id":"W3022649854","doi":"10.3847/1538-4357/ab8eaf","title":"SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). IV. Spatial Clustering and Halo Masses of Submillimeter Galaxies","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Herzberg Institute of Astrophysics; University of Victoria; University of British Columbia","funders":"Science and Technology Facilities Council; Ministry of Science and Technology, Taiwan","keywords":"Galaxy; Redshift; Halo; Hubble Deep Field; Photometry (optics); Bolometer; Active galactic nucleus; Radio galaxy","score_opus":0.01777374253682585,"score_gpt":0.23269802507037193,"score_spread":0.2149242825335461,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3022649854","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.986545,0.000098596916,0.00040275021,0.000046226076,0.000004198483,0.000032584525,0.010177573,0.00008249646,0.0026105137],"genre_scores_gemma":[0.9743663,0.000055442153,0.0012064136,0.00004077224,0.000012967299,0.000022887976,0.023037978,0.000024970486,0.0012322963],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998903,0.000012212501,0.0000069040198,0.000026658687,0.000025325293,0.00003857851],"domain_scores_gemma":[0.9995352,0.000030409616,0.00015593879,0.000069723574,0.00007524823,0.00013340122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021828429,0.0002436741,0.00014950075,0.0019866866,0.00024585822,0.0003970062,0.00024653142,0.0001538972,0.0018862105],"category_scores_gemma":[0.00043867846,0.00011682884,0.00031968995,0.0015105553,0.00013365329,0.00021670392,0.00041504842,0.0001819973,0.0006785868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000080145655,0.000040494397,0.9812913,0.00001794698,0.00005242229,0.000072710725,0.00005182949,0.0007504149,0.0047507356,0.00020393958,0.0038413075,0.008846676],"study_design_scores_gemma":[0.000004159314,0.00000612218,0.99782443,0.0000023157932,0.000005798116,0.000026537726,0.000026901189,0.00097607105,0.00034361877,0.00003454929,0.0007478345,0.0000018039921],"about_ca_topic_score_codex":0.016770734,"about_ca_topic_score_gemma":0.032790188,"teacher_disagreement_score":0.016770734,"about_ca_system_score_codex":0.00025329107,"about_ca_system_score_gemma":0.00024185023,"threshold_uncertainty_score":0.033346236},"labels":[],"label_agreement":null},{"id":"W3023240439","doi":"10.3847/1538-4357/abd62b","title":"Discovering New Strong Gravitational Lenses in the DESI Legacy Imaging Surveys","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":92,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Perimeter Institute","funders":"Lawrence Berkeley National Laboratory; SLAC National Accelerator Laboratory; Fermilab; High Energy Physics; Office of Science; Institut de Física d'Altes Energies; Science and Technology Facilities Council; University College London; National Energy Research Scientific Computing Center; Deutsche Forschungsgemeinschaft; University of Portsmouth; Ohio State University; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; University of Sussex; University of Pennsylvania; Argonne National Laboratory; U.S. Department of Energy; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University of Chicago; National Science Foundation","keywords":"Physics; Astronomy; Gravitational lens; Gravitation; Astrophysics; Galaxy; Redshift","score_opus":0.014580580197893723,"score_gpt":0.26965268353989974,"score_spread":0.25507210334200603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3023240439","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911499,0.00051776756,0.0025296742,0.00019413413,0.000009974436,0.000014469586,0.0033023315,0.0002508947,0.0020309947],"genre_scores_gemma":[0.98371625,0.00020108343,0.0065239295,0.00007538263,0.00002807853,0.000008485658,0.008427959,0.00005351065,0.00096535834],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996369,0.000054254844,0.00001532288,0.00010241175,0.00011296319,0.00007806508],"domain_scores_gemma":[0.9987924,0.00028256085,0.00033350717,0.00014911653,0.00019478568,0.0002475429],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009369713,0.0003301672,0.00024164462,0.0019736446,0.0003800863,0.0007596177,0.00033293452,0.00020114124,0.0015852571],"category_scores_gemma":[0.001724262,0.00021035389,0.00040246584,0.0013301211,0.00027894965,0.00044181422,0.0010119481,0.00031175805,0.0004896683],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017759771,0.000074429685,0.9298009,0.000094991694,0.0002401882,0.00029244268,0.0003416526,0.006225325,0.007826998,0.0011859273,0.0069595245,0.04678008],"study_design_scores_gemma":[0.000026331596,0.000052530988,0.9703317,0.00003187485,0.000071384115,0.0001510598,0.00030705193,0.015373365,0.0031356055,0.00077396486,0.009718888,0.000026275806],"about_ca_topic_score_codex":0.012562961,"about_ca_topic_score_gemma":0.03950293,"teacher_disagreement_score":0.012562961,"about_ca_system_score_codex":0.0005625147,"about_ca_system_score_gemma":0.00043501722,"threshold_uncertainty_score":0.024979651},"labels":[],"label_agreement":null},{"id":"W3023462503","doi":"10.3847/1538-4357/ac01c6","title":"Resolving the Emission Regions of the Crab Pulsar’s Giant Pulses","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"","keywords":"Physics; Crab Pulsar; Pulsar; Scintillation; Astrophysics; Pulse (music); Scattering; Amplitude; Crab Nebula; Sky; Optics; Detector","score_opus":0.020296898005150887,"score_gpt":0.31896126379766676,"score_spread":0.2986643657925159,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3023462503","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972464,0.00016077196,0.001267018,0.000021595568,0.0000033882916,0.0000018002169,0.00019726352,0.00003244972,0.001069308],"genre_scores_gemma":[0.99782264,0.00005527726,0.0014689626,0.000012036993,0.000006546522,0.0000025295888,0.00036665692,0.000017109405,0.0002482759],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996305,0.0000035136977,0.0000016840123,0.000011171984,0.000010621484,0.000010028044],"domain_scores_gemma":[0.9997811,0.00006340586,0.000060731676,0.000029601475,0.000031990956,0.00003320663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012367612,0.00012339317,0.00016449855,0.00078689057,0.00016764698,0.00033293708,0.00014343702,0.00015520983,0.0010279347],"category_scores_gemma":[0.0004665638,0.0001409304,0.00009996663,0.00053889427,0.00012313046,0.00020982727,0.00037563246,0.00020418738,0.00018846148],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049902615,0.00007973399,0.23743778,0.00008984075,0.00009798529,0.00061338657,0.00034849133,0.0031983312,0.71286446,0.000994376,0.0007069104,0.043069717],"study_design_scores_gemma":[0.00002002504,0.00009056728,0.9597741,0.00001040708,0.00002949062,0.000625756,0.00011759103,0.006328772,0.030596385,0.00035775724,0.0020341824,0.00001498964],"about_ca_topic_score_codex":0.00088419183,"about_ca_topic_score_gemma":0.0023988718,"teacher_disagreement_score":0.0010279347,"about_ca_system_score_codex":0.00016275486,"about_ca_system_score_gemma":0.000085394444,"threshold_uncertainty_score":0.0034388304},"labels":[],"label_agreement":null},{"id":"W3024084526","doi":"10.3847/1538-4357/ab91ad","title":"Diffusion Coefficients in the Envelopes of White Dwarfs","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"U.S. Department of Energy","keywords":"White dwarf; Diffusion; Context (archaeology); Stellar classification; Plasma; Helium; Ionization; Hydrogen","score_opus":0.013545573413770001,"score_gpt":0.22183237891492918,"score_spread":0.2082868055011592,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3024084526","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.979391,0.00037803035,0.015819386,0.00009233312,0.00001978449,0.000014254937,0.00013795577,0.000130693,0.0040166434],"genre_scores_gemma":[0.9976943,0.00015236977,0.0012633554,0.00001292818,0.0000037766079,0.0000056436334,0.000074234726,0.000034108514,0.0007592858],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999057,0.000013834437,0.0000054569427,0.000023309005,0.000030992527,0.000020719679],"domain_scores_gemma":[0.9995695,0.00020393195,0.000055183667,0.000035408193,0.00009292022,0.000043008735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035557078,0.00029994873,0.00028536172,0.00062234025,0.00034643142,0.0007122485,0.00053812895,0.00042288122,0.00071208045],"category_scores_gemma":[0.002060294,0.00021541084,0.00041913695,0.0003077953,0.00040809077,0.0006267683,0.0005608885,0.00031423537,0.00018164761],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022056412,0.00007346295,0.072608024,0.00018611872,0.000103808634,0.0008260068,0.00088965613,0.75669765,0.10958377,0.043420345,0.00079632277,0.014594318],"study_design_scores_gemma":[0.000033912907,0.00003239061,0.019003218,0.000015271813,0.000026803047,0.00019209617,0.00011360674,0.9533815,0.020399535,0.0048968387,0.0018737167,0.00003115744],"about_ca_topic_score_codex":0.008828349,"about_ca_topic_score_gemma":0.0030841231,"teacher_disagreement_score":0.008828349,"about_ca_system_score_codex":0.0008744602,"about_ca_system_score_gemma":0.0003697808,"threshold_uncertainty_score":0.017553926},"labels":[],"label_agreement":null},{"id":"W3024277966","doi":"10.3847/1538-4357/abbacd","title":"A Measurement of the CMB E-mode Angular Power Spectrum at Subdegree Scales from 670 Square Degrees of POLARBEAR Data","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Advanced Research; Dalhousie University","funders":"Gordon and Betty Moore Foundation; Simons Foundation; Science and Technology Facilities Council; Agence Nationale de la Recherche; National Science Foundation","keywords":"Physics; Cosmic microwave background; Spectral density; Lambda; Planck; Multipole expansion; Astrophysics; Polarization (electrochemistry); Hubble's law; Cosmic background radiation; Cosmology; Dark energy; Quantum mechanics; Anisotropy; Statistics","score_opus":0.025309322616623626,"score_gpt":0.252414295276177,"score_spread":0.22710497265955334,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3024277966","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98511744,0.00011708534,0.0052702706,0.00006587867,0.000017418393,0.00001000987,0.0048048683,0.00014642105,0.0044506365],"genre_scores_gemma":[0.9922455,0.000081040016,0.0029316747,0.000024639747,0.000024018404,0.000013352317,0.004271057,0.00003083851,0.00037788006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997687,0.000039407874,0.000009139804,0.00006300225,0.00008362824,0.00003608938],"domain_scores_gemma":[0.99939466,0.0001635524,0.00012890519,0.00010264446,0.0001463522,0.0000638848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003236842,0.0003146683,0.00014190911,0.0011364969,0.0001851175,0.00036125357,0.00018313437,0.00020240272,0.0015891289],"category_scores_gemma":[0.00085213705,0.00019008771,0.00014589414,0.0010463324,0.00015500706,0.0002762169,0.00040561997,0.00031788193,0.0006029739],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005391729,0.00015141472,0.8254824,0.00010571398,0.00022881523,0.00023277725,0.0002696614,0.0051679364,0.10656731,0.0014207956,0.003289817,0.056544174],"study_design_scores_gemma":[0.000010031205,0.000048282076,0.97549236,0.000012515101,0.000031224605,0.00015495534,0.00007890267,0.0040574674,0.016797394,0.00024177486,0.0030579884,0.00001696885],"about_ca_topic_score_codex":0.0021189959,"about_ca_topic_score_gemma":0.0032550925,"teacher_disagreement_score":0.0021189959,"about_ca_system_score_codex":0.00012915692,"about_ca_system_score_gemma":0.00007863875,"threshold_uncertainty_score":0.0053161383},"labels":[],"label_agreement":null},{"id":"W3025362700","doi":"10.3847/1538-4357/aba61c","title":"Velocity Dispersions of Massive Quiescent Galaxies from Weak Lensing and Spectroscopy*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Japan Society for the Promotion of Science; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Japan Science and Technology Agency; Ohio State University; Brookhaven National Laboratory; Academia Sinica; U.S. Department of Energy; Ministry of Education, Culture, Sports, Science and Technology; Princeton University; New Mexico State University; Smithsonian Institution; Alfred P. Sloan Foundation; York University; Toray Science Foundation; National Science Foundation","keywords":"Velocity dispersion; Dark matter; Galaxy; Weak gravitational lensing; Halo; Redshift; Dark matter halo","score_opus":0.009580610534011776,"score_gpt":0.21043085507866643,"score_spread":0.20085024454465467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3025362700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983834,0.00012931305,0.00042817066,0.00001290016,0.0000019876836,0.0000022200854,0.0002785461,0.000038610993,0.0007247928],"genre_scores_gemma":[0.99913186,0.000022590963,0.00021322047,0.0000056249332,0.0000059766767,0.0000011620422,0.00053370657,0.000005070086,0.000080853366],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978787,0.000027968152,0.000018715715,0.00006972564,0.000059742368,0.000036087662],"domain_scores_gemma":[0.9982798,0.00025888043,0.0006835249,0.00020000171,0.00015922125,0.0004185864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006557107,0.00033600745,0.0002792434,0.002854906,0.0002405924,0.00086397945,0.00024065412,0.00024029185,0.00081885577],"category_scores_gemma":[0.0018552719,0.00021647738,0.00022915116,0.0012948556,0.00043561042,0.00044779855,0.0007713987,0.00016063433,0.00025779151],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017882562,0.00003360156,0.96457434,0.000024865878,0.000098269666,0.00007799836,0.0003578097,0.00082079513,0.022645818,0.0005782645,0.00021152673,0.0103977285],"study_design_scores_gemma":[0.0000051753073,0.00004244591,0.99536633,0.0000041485378,0.000020421396,0.0000750723,0.00006434551,0.0016140364,0.0023109685,0.00021403797,0.0002752819,0.000007786442],"about_ca_topic_score_codex":0.0030992182,"about_ca_topic_score_gemma":0.0037913406,"teacher_disagreement_score":0.0030992182,"about_ca_system_score_codex":0.00041298682,"about_ca_system_score_gemma":0.00010451568,"threshold_uncertainty_score":0.006162405},"labels":[],"label_agreement":null},{"id":"W3025807255","doi":"10.3847/1538-4357/ab8d1f","title":"On the Paradoxical Impact of Blending by Red Clump Giants","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Mount Saint Vincent University","funders":"","keywords":"Red clump; Cepheid variable; Large Magellanic Cloud; Stars; Cosmic distance ladder; Red-giant branch; Parallax; Metallicity; Apparent magnitude","score_opus":0.017474982739885653,"score_gpt":0.2487061335663815,"score_spread":0.23123115082649584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3025807255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.986267,0.0002506853,0.002735899,0.00089240994,0.000039617258,0.0000062782915,0.00013077055,0.00018967634,0.009487676],"genre_scores_gemma":[0.99905795,0.000047787795,0.00033123788,0.00010522899,0.0000129827795,0.0000017421332,0.00004218472,0.00004380042,0.0003571787],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980885,0.00006470381,0.0000061829105,0.000042290496,0.000039112132,0.000038886443],"domain_scores_gemma":[0.998992,0.000457663,0.00014264457,0.00013064596,0.000088257715,0.0001887772],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005941208,0.00033364407,0.0004320942,0.00032709373,0.0005902925,0.0013054232,0.0005700231,0.00044615183,0.0034113473],"category_scores_gemma":[0.0032301715,0.00015519517,0.000339782,0.00031291877,0.0008641787,0.0012040668,0.0011204366,0.0007154758,0.0003573365],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017810632,0.00032424252,0.4316404,0.00032625854,0.00054397434,0.0035093834,0.002504071,0.3121996,0.035670802,0.124887265,0.016013915,0.07059906],"study_design_scores_gemma":[0.00030024588,0.0005078506,0.1957861,0.00011075544,0.00027138824,0.00071802555,0.001856508,0.6910011,0.0097784875,0.08755006,0.011985756,0.00013369686],"about_ca_topic_score_codex":0.006450159,"about_ca_topic_score_gemma":0.0054942905,"teacher_disagreement_score":0.006450159,"about_ca_system_score_codex":0.0006258085,"about_ca_system_score_gemma":0.00019248427,"threshold_uncertainty_score":0.012825191},"labels":[],"label_agreement":null},{"id":"W3026106441","doi":"10.3847/1538-4357/ab9953","title":"PHANGS CO Kinematics: Disk Orientations and Rotation Curves at 150 pc Resolution","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":153,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Galaxy rotation curve; Rotation (mathematics); Kinematics; Orientation (vector space); Amplitude; Mass distribution; Galaxy; Radial velocity","score_opus":0.017525593467642767,"score_gpt":0.26422986529795567,"score_spread":0.2467042718303129,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3026106441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98586047,0.00023778784,0.006832356,0.000040693234,0.000012946628,0.000013354758,0.0021551258,0.0008400496,0.004007203],"genre_scores_gemma":[0.9927918,0.0000715246,0.004831863,0.000007068615,0.000010695422,0.0000070572855,0.0018111883,0.00007823935,0.0003905496],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987197,0.000015242363,0.0000059626686,0.00004632485,0.000033110005,0.000027375721],"domain_scores_gemma":[0.9995347,0.000056767392,0.0001171967,0.00011159869,0.000108477136,0.000071266804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002833515,0.00024544576,0.00018409817,0.0014312712,0.00023232105,0.00046694995,0.00021487544,0.00016464447,0.0017131976],"category_scores_gemma":[0.000852232,0.00014383488,0.0002255447,0.0009499324,0.00014862802,0.0002339176,0.000269993,0.00017116762,0.0007948951],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029519096,0.0001082899,0.7023434,0.00011466123,0.00013387024,0.00024194737,0.0005968022,0.020067127,0.14537622,0.0011854756,0.0031833167,0.12635358],"study_design_scores_gemma":[0.000006723389,0.00003247322,0.96929675,0.000008140284,0.0000147978835,0.00014617013,0.0000752461,0.019348158,0.008454549,0.0002296342,0.0023705885,0.000016746815],"about_ca_topic_score_codex":0.004563113,"about_ca_topic_score_gemma":0.005872845,"teacher_disagreement_score":0.004563113,"about_ca_system_score_codex":0.0003194368,"about_ca_system_score_gemma":0.00015101429,"threshold_uncertainty_score":0.009073138},"labels":[],"label_agreement":null},{"id":"W3026700980","doi":"10.3847/1538-4357/ab9634","title":"Measuring HERA's Primary Beam in Situ: Methodology and First Results","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"HERA; Physics; Reionization; Telescope; Beam (structure); Cosmology; Optics; Astrophysics; Particle physics; Redshift; Galaxy","score_opus":0.060228703465869435,"score_gpt":0.24534754727452918,"score_spread":0.18511884380865973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3026700980","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.61376756,0.00028195363,0.37216082,0.00017001783,0.000031335443,0.00038663155,0.0036613867,0.002378663,0.0071616746],"genre_scores_gemma":[0.8401011,0.00014849643,0.1554611,0.00006877845,0.000019417845,0.00020433785,0.0025379378,0.0002810061,0.0011777411],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9990274,0.00039496206,0.000039109113,0.00021589073,0.00023864357,0.00008404777],"domain_scores_gemma":[0.9975038,0.00077568064,0.00022457643,0.00078725815,0.0005965567,0.00011203582],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020345768,0.0006610558,0.00033032778,0.0005841703,0.00052117184,0.00084329693,0.00083165494,0.0007185021,0.0025814641],"category_scores_gemma":[0.003427587,0.000339943,0.0004812392,0.001139306,0.00036589248,0.0006915695,0.0008879623,0.00045025809,0.0012809505],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010948635,0.0029871452,0.38017318,0.0005077873,0.000498085,0.00054221466,0.0009031876,0.17583905,0.15845223,0.010339984,0.004189988,0.26447225],"study_design_scores_gemma":[0.00020661995,0.0015400153,0.18132351,0.000076262535,0.00024143998,0.00082584354,0.0007455345,0.58427095,0.20843133,0.008344922,0.01374499,0.00024851895],"about_ca_topic_score_codex":0.0066420184,"about_ca_topic_score_gemma":0.0055126874,"teacher_disagreement_score":0.0066420184,"about_ca_system_score_codex":0.00069956185,"about_ca_system_score_gemma":0.00030626205,"threshold_uncertainty_score":0.01320672},"labels":[],"label_agreement":null},{"id":"W3029308127","doi":"10.3847/1538-4357/abb464","title":"Systematically Measuring Ultradiffuse Galaxies in H i: Results from the Pilot Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Coma Cluster; Galaxy; Coma (optics); Surface brightness; Hydrogen line; Baryon; Telescope; Line (geometry)","score_opus":0.05565680301341617,"score_gpt":0.23710570997955213,"score_spread":0.18144890696613597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3029308127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990558,0.000038989932,0.0001703795,0.000021038024,0.0000015687025,0.000022521443,0.00037761938,0.000015232885,0.0002968882],"genre_scores_gemma":[0.99846065,0.00003395931,0.0003553957,0.000029652085,0.000004763084,0.000016173548,0.00094198773,0.000005922877,0.00015157627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989095,0.00038658,0.00004934068,0.00019866819,0.00024251272,0.00021339774],"domain_scores_gemma":[0.9970849,0.00038510666,0.00060894125,0.00048334742,0.0005071397,0.0009304915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015155663,0.000410256,0.00031306795,0.0013975499,0.00040068536,0.0005037884,0.0005175363,0.00022562449,0.00047318763],"category_scores_gemma":[0.001997592,0.00022376556,0.0002823623,0.0008447796,0.00060007523,0.00035848995,0.0013715841,0.0002999905,0.00025043162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015828192,0.00008558097,0.98925334,0.0000139330805,0.000027021368,0.00008786457,0.0006292428,0.000074854135,0.002998227,0.000039734412,0.00025659346,0.006375293],"study_design_scores_gemma":[0.0000076951,0.00011653096,0.99854624,0.00000320044,0.000010171307,0.00007450126,0.00029922105,0.00009997209,0.00043087007,0.000013779232,0.00039366464,0.000004088685],"about_ca_topic_score_codex":0.015406748,"about_ca_topic_score_gemma":0.03266064,"teacher_disagreement_score":0.015406748,"about_ca_system_score_codex":0.00041600506,"about_ca_system_score_gemma":0.00030322105,"threshold_uncertainty_score":0.030634165},"labels":[],"label_agreement":null},{"id":"W3030742755","doi":"10.3847/1538-4357/ab9b8d","title":"The 100 pc White Dwarf Sample in the SDSS Footprint","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":143,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Los Alamos National Laboratory; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; Dartmouth College; Ohio State University; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"White dwarf; Sky; Population; Stars; Mass distribution; Massive compact halo object; Blue dwarf; Main sequence; White (mutation)","score_opus":0.02022864535878025,"score_gpt":0.2351940694081799,"score_spread":0.21496542404939967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3030742755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9821425,0.000112514615,0.00065688306,0.0000374571,0.00000395397,0.000012651594,0.014913885,0.00025932895,0.0018607931],"genre_scores_gemma":[0.93675697,0.000118017815,0.0018271769,0.000048782273,0.000011844025,0.00002499456,0.059215922,0.0000946241,0.0019015984],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997713,0.000018956938,0.000008850333,0.000067915644,0.000074267424,0.000058810798],"domain_scores_gemma":[0.999645,0.000029545386,0.000059602207,0.000103924605,0.00006641046,0.00009558174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026165717,0.00022536972,0.0002083502,0.0010708612,0.0003248475,0.00038810258,0.00023250254,0.00014997247,0.0022155652],"category_scores_gemma":[0.00046112365,0.000117467716,0.00025677352,0.0014381607,0.00013545231,0.00022951436,0.0005808389,0.00011019366,0.0013666677],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028828948,0.000096861775,0.9249716,0.000065651875,0.00011130885,0.0003782354,0.00060690416,0.0015787601,0.024597742,0.0005935487,0.008593316,0.038117822],"study_design_scores_gemma":[0.0000085592155,0.000017046044,0.9890766,0.0000038917383,0.00001157097,0.00010275689,0.00016684657,0.0010922365,0.0014178699,0.00010741669,0.0079909405,0.0000042922647],"about_ca_topic_score_codex":0.01609687,"about_ca_topic_score_gemma":0.02329565,"teacher_disagreement_score":0.01609687,"about_ca_system_score_codex":0.000276224,"about_ca_system_score_gemma":0.0002850319,"threshold_uncertainty_score":0.032006323},"labels":[],"label_agreement":null},{"id":"W3030786681","doi":"","title":"Space Telescope Imaging Spectrograph Long-Slit Spectroscopy of the Narrow-Line Region of NGC 4151","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Space Telescope Imaging Spectrograph; Astrophysics; Doubly ionized oxygen; Outflow; Galaxy; Astronomy; Emission spectrum; Radial velocity; Spectroscopy; Line (geometry); Spectral line; Stars; Hubble space telescope; Geometry","score_opus":0.00813617484509918,"score_gpt":0.23500069788022,"score_spread":0.2268645230351208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3030786681","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930997,0.00013079803,0.00039548814,0.000048190148,0.00000778439,0.000010757599,0.0025231298,0.00012960083,0.0036545452],"genre_scores_gemma":[0.9868579,0.00015091429,0.001671602,0.000081580416,0.000013936587,0.000023616964,0.007671804,0.00002485712,0.0035038933],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998815,0.000011014518,0.000009103827,0.00003706059,0.000038473972,0.000022832648],"domain_scores_gemma":[0.999501,0.000044610413,0.00015455995,0.000065298416,0.000095404146,0.00013911887],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022051299,0.0002278162,0.00018037455,0.0012544923,0.00044747262,0.00039157787,0.00021565252,0.0002741079,0.0032433262],"category_scores_gemma":[0.0003500052,0.0001257871,0.00015996501,0.00091977016,0.00012127562,0.00024562553,0.00029152204,0.0002389683,0.00062891707],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043037318,0.00015248418,0.7946603,0.000113344395,0.00014050529,0.00056378596,0.0010992769,0.0006734125,0.17289251,0.00042473213,0.0038423184,0.02500694],"study_design_scores_gemma":[0.0000048496354,0.00002812964,0.9961713,0.0000040630152,0.000013906641,0.000088008004,0.000077308905,0.00024544552,0.0017214592,0.000023324583,0.0016194067,0.0000028116935],"about_ca_topic_score_codex":0.008122819,"about_ca_topic_score_gemma":0.020770354,"teacher_disagreement_score":0.008122819,"about_ca_system_score_codex":0.0003895803,"about_ca_system_score_gemma":0.00015842987,"threshold_uncertainty_score":0.01615113},"labels":[],"label_agreement":null},{"id":"W3030895789","doi":"10.3847/1538-4357/ab8a44","title":"Discovery of a 2.8 s Pulsar in a 2 Day Orbit High-mass X-Ray Binary Powering the Ultraluminous X-Ray Source ULX-7 in M51","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":151,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; New York University Abu Dhabi; INAF - Osservatorio Astrofisico di Catania; York University; National Aeronautics and Space Administration","keywords":"Pulsar; Luminosity; Neutron star; Galaxy; Orbit (dynamics); X-ray binary; Spiral galaxy; Binary star; Amplitude","score_opus":0.010847147397718734,"score_gpt":0.21499979850588646,"score_spread":0.20415265110816772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3030895789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991702,0.00008983979,0.00015652957,0.000025851168,0.000009443019,0.0000040847835,0.000046920366,0.000011108253,0.00048612113],"genre_scores_gemma":[0.99912995,0.000029428757,0.00034721647,0.00003669247,0.000018925655,0.000004979529,0.00013331533,0.0000040977793,0.00029542518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990773,0.000008135461,0.000005720044,0.00003502943,0.000018787312,0.00002450575],"domain_scores_gemma":[0.9996921,0.000028882729,0.00012789754,0.000044428754,0.000030165704,0.000076593504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018953696,0.00020997276,0.0002773146,0.0007097289,0.0005353323,0.0006682,0.0002912059,0.0007704907,0.0010138265],"category_scores_gemma":[0.00037658258,0.00021566526,0.000252313,0.00035850893,0.0003272625,0.00022591143,0.0007806765,0.000441062,0.0004473506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006579984,0.00017144758,0.6389688,0.000080784455,0.000102669146,0.010550311,0.0011554924,0.00023060323,0.32917726,0.0008677965,0.0005644025,0.017472383],"study_design_scores_gemma":[0.000016736949,0.00036040472,0.98674184,0.00001594733,0.00003365631,0.0037804488,0.00019080077,0.00044196678,0.006028389,0.0001433465,0.0022334203,0.000012989395],"about_ca_topic_score_codex":0.000368428,"about_ca_topic_score_gemma":0.0007036187,"teacher_disagreement_score":0.0010138265,"about_ca_system_score_codex":0.0002575618,"about_ca_system_score_gemma":0.00008517357,"threshold_uncertainty_score":0.003391564},"labels":[],"label_agreement":null},{"id":"W3031258807","doi":"10.3847/1538-4357/ab9631","title":"Multiwavelength Observations of 2HWC J1928+177: Dark Accelerator or New TeV Gamma-Ray Binary?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Goddard Space Flight Center; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; National Research Foundation; Office of Science; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; National Research Foundation of Korea; Universities Space Research Association; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Science Foundation","keywords":"Pulsar; Pulsar wind nebula; Supernova remnant; Nebula; Cherenkov radiation; Observatory; Supernova; Point source","score_opus":0.039715920409168305,"score_gpt":0.24811207249748518,"score_spread":0.20839615208831688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3031258807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944084,0.00019981233,0.00018507274,0.0000836193,0.000015608553,0.000013673654,0.0013511962,0.000078913174,0.0036635303],"genre_scores_gemma":[0.9943547,0.00009490948,0.0008929319,0.00011085593,0.000040977633,0.000017270362,0.0028638802,0.00005332751,0.0015711488],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999393,0.0000024489736,0.0000023784348,0.000020786918,0.000014644264,0.000020444515],"domain_scores_gemma":[0.99981326,0.00001099302,0.000042234456,0.000021941707,0.00002746281,0.000084276486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000122594,0.00018152884,0.00031289132,0.0009873623,0.0005072566,0.00048340834,0.0002993411,0.0002839792,0.0027030949],"category_scores_gemma":[0.0001225558,0.00017382005,0.00016951853,0.000577516,0.00014054656,0.0001543463,0.0004728245,0.00036604653,0.0008219821],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058043393,0.00021573337,0.60707295,0.0001501991,0.00019892285,0.004665237,0.00053139054,0.0005120309,0.34808975,0.0006015296,0.009133306,0.02824851],"study_design_scores_gemma":[0.00002786978,0.00005090198,0.98829216,0.000009883744,0.000034784476,0.00071031525,0.00013842624,0.0005163929,0.0042892452,0.000095413096,0.0058214967,0.000013048023],"about_ca_topic_score_codex":0.0059021846,"about_ca_topic_score_gemma":0.018955186,"teacher_disagreement_score":0.0059021846,"about_ca_system_score_codex":0.0003489572,"about_ca_system_score_gemma":0.0001360654,"threshold_uncertainty_score":0.011735618},"labels":[],"label_agreement":null},{"id":"W3032818697","doi":"10.1086/510202","title":"Broad Absorption Line Variability in Repeat Quasar Observations from the Sloan Digital Sky Survey","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Quasar; Sky; Astrophysics; Emission spectrum; Spectral line; Physics; Equivalent width; Rest frame; Absorption spectroscopy; Trough (economics); Astronomy; Optics; Galaxy; Redshift","score_opus":0.019940922381458507,"score_gpt":0.23602746976853534,"score_spread":0.21608654738707683,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3032818697","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952066,0.000013317639,0.00008277801,0.0000032908467,3.994619e-7,0.0000013481351,0.0002953409,0.000004346819,0.00007861143],"genre_scores_gemma":[0.99855787,0.000012389566,0.0000979723,0.000002530193,0.0000014886625,0.000002543841,0.0012580523,0.0000021620865,0.00006484634],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982625,0.000030231562,0.000013081375,0.000043816926,0.000047696372,0.000038904447],"domain_scores_gemma":[0.9991172,0.00013489951,0.0003887413,0.00008612648,0.00014718289,0.00012581071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000313392,0.00014188395,0.00015093785,0.0010050659,0.00018800687,0.00034153348,0.00015803262,0.00010549574,0.0003271034],"category_scores_gemma":[0.00082595693,0.000084737316,0.0001711025,0.0007882783,0.0001971352,0.00018706148,0.00036009177,0.00013709228,0.00010257463],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000583764,0.000026433938,0.993814,0.000005877282,0.00006162984,0.00006482764,0.00011779758,0.00054322626,0.0026989926,0.000041645875,0.00016293408,0.0024043175],"study_design_scores_gemma":[0.0000011324421,0.0000098027085,0.99923396,4.523187e-7,0.0000043210002,0.000032151347,0.000028675908,0.0004604438,0.00013076788,0.000007717537,0.00008924664,0.0000013342958],"about_ca_topic_score_codex":0.011881128,"about_ca_topic_score_gemma":0.022244819,"teacher_disagreement_score":0.011881128,"about_ca_system_score_codex":0.00028518224,"about_ca_system_score_gemma":0.0001239998,"threshold_uncertainty_score":0.023623943},"labels":[],"label_agreement":null},{"id":"W3032914308","doi":"10.3847/1538-4357/ab8f28","title":"The Flare-dominated Accretion Mode of a Radio-bright Candidate Transitional Millisecond Pulsar","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Millisecond pulsar; Neutron star; Millisecond; Flare; Accretion (finance); Luminosity; Telescope; Amplitude; Pulsar","score_opus":0.008530370029757926,"score_gpt":0.22312258892687092,"score_spread":0.214592218897113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3032914308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99961615,0.000026056056,0.00005690124,0.00000676215,0.0000013531034,0.0000013206536,0.000028296638,0.0000058614132,0.0002573196],"genre_scores_gemma":[0.9995042,0.000016337912,0.00013850746,0.000015094613,0.0000036191232,0.0000025059107,0.00013362615,0.0000020848047,0.00018412099],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996376,0.0000032542098,0.000001989198,0.0000080166055,0.000007938767,0.000014898042],"domain_scores_gemma":[0.99986196,0.000010091237,0.00005590245,0.000010712429,0.000017118706,0.000044173838],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008536156,0.00012368224,0.00019816191,0.00057830254,0.0003590428,0.0004081326,0.00026490353,0.0001878712,0.00088261813],"category_scores_gemma":[0.00014859246,0.0000771283,0.00011557884,0.00028018426,0.00018233409,0.00011181077,0.00030745775,0.00016399709,0.00021298561],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004280578,0.0001398947,0.83502305,0.000039167462,0.000047764657,0.0024717315,0.0006366004,0.00014332822,0.14507662,0.00025459318,0.0006207248,0.015118531],"study_design_scores_gemma":[0.000011518237,0.00017470076,0.99275595,0.000005723718,0.000015562386,0.0018703856,0.0002937057,0.0003827615,0.003089274,0.00007349339,0.0013202471,0.00000657681],"about_ca_topic_score_codex":0.0015811868,"about_ca_topic_score_gemma":0.0033593583,"teacher_disagreement_score":0.0015811868,"about_ca_system_score_codex":0.00019403787,"about_ca_system_score_gemma":0.000074751646,"threshold_uncertainty_score":0.0031439662},"labels":[],"label_agreement":null},{"id":"W3033287669","doi":"10.3847/1538-4357/ab91b5","title":"Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XI. Accretion Disk Reverberation Mapping of Mrk 142","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Active galactic nucleus; Supermassive black hole; Accretion (finance); Observatory; Reverberation mapping; Accretion disc; Spectral line; Flux (metallurgy); Extrapolation","score_opus":0.015472828697415404,"score_gpt":0.22711073509551463,"score_spread":0.21163790639809923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3033287669","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991123,0.00014235188,0.0002406438,0.000008425681,0.0000021973412,0.0000051999136,0.00014657565,0.000012699086,0.00032964273],"genre_scores_gemma":[0.9989881,0.000034603767,0.00050875306,0.0000073461124,0.000005376976,0.0000034198029,0.0002972256,0.000004996716,0.00015020746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998952,0.000013172364,0.0000064200776,0.00004099833,0.000020545694,0.000023693212],"domain_scores_gemma":[0.99972147,0.000023567729,0.00015143081,0.000027223265,0.000027494802,0.00004871049],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023249278,0.0003564067,0.00026245243,0.0007898946,0.0003461744,0.00044869393,0.00026756368,0.00021201228,0.00065474096],"category_scores_gemma":[0.0004309067,0.00015547303,0.00023415011,0.00044598323,0.00020737352,0.00025851242,0.0005100564,0.0001848882,0.00029201747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032254274,0.00007675681,0.8944766,0.000055185188,0.000077020275,0.0012687462,0.0004248564,0.0005095757,0.09230725,0.00014702961,0.0001830981,0.010151374],"study_design_scores_gemma":[0.000005305943,0.000049948194,0.9962341,0.0000043861223,0.000012347339,0.00046635448,0.000100084864,0.00050103967,0.0022130774,0.000042829102,0.00036638338,0.000004222475],"about_ca_topic_score_codex":0.0022848882,"about_ca_topic_score_gemma":0.004714378,"teacher_disagreement_score":0.0022848882,"about_ca_system_score_codex":0.00018263685,"about_ca_system_score_gemma":0.00008539095,"threshold_uncertainty_score":0.0045431852},"labels":[],"label_agreement":null},{"id":"W3033479311","doi":"10.3847/1538-4357/abec3d","title":"EMPRESS. II. Highly Fe-enriched Metal-poor Galaxies with ∼1.0 (Fe/O)<sub>⊙</sub> and 0.02 (O/H)<sub>⊙</sub>: Possible Traces of Supermassive (&gt;300 M <sub>⊙</sub>) Stars in Early Galaxies* † ‡","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Japan Society for the Promotion of Science; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; National Research Foundation; High Energy Accelerator Research Organization; Max-Planck-Gesellschaft; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; National Astronomical Observatory of Japan; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; W. M. Keck Foundation; Space Telescope Science Institute; Los Alamos National Laboratory; Johns Hopkins University; Princeton University; National Central University; Gordon and Betty Moore Foundation; Queen's University Belfast; Eötvös Loránd Tudományegyetem; Academia Sinica; California Institute of Technology; Durham University; Japan Science and Technology Agency; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Nucleosynthesis; Galaxy; Abundance (ecology); Supernova; Stars; Oxygen; Abundance of the chemical elements; Astronomy","score_opus":0.006491500348729626,"score_gpt":0.19370029219514392,"score_spread":0.1872087918464143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3033479311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944622,0.00014734104,0.00014631187,0.000024189521,0.0000019532197,0.0000062752506,0.0025952868,0.00004234738,0.0025741325],"genre_scores_gemma":[0.99035066,0.0001491832,0.000566574,0.000031482443,0.000008987499,0.000010628603,0.0063587124,0.000017257506,0.002506368],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999454,0.0000044520884,0.000003896825,0.000019131048,0.000009604477,0.00001742136],"domain_scores_gemma":[0.99974245,0.000022152146,0.00012765174,0.000031757183,0.000023498404,0.000052495645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001263056,0.00022054053,0.0001438283,0.00070708554,0.0001947849,0.00040318375,0.00018277814,0.00013847495,0.0017806236],"category_scores_gemma":[0.00020834425,0.0001031872,0.00012592475,0.0004534705,0.00017093308,0.00032407203,0.00052483263,0.00015154122,0.00055953837],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024759737,0.00004016977,0.9740384,0.00004444319,0.000031360505,0.00037273095,0.00028629723,0.0001572884,0.006725105,0.00029998083,0.001733017,0.016023532],"study_design_scores_gemma":[0.0000017073759,0.000017047427,0.9978452,0.0000024999267,0.000007074211,0.00015508223,0.000080267535,0.00007290892,0.0006459472,0.000017143962,0.0011542772,8.6694763e-7],"about_ca_topic_score_codex":0.002217836,"about_ca_topic_score_gemma":0.003179934,"teacher_disagreement_score":0.002217836,"about_ca_system_score_codex":0.00013320353,"about_ca_system_score_gemma":0.00008085846,"threshold_uncertainty_score":0.005956769},"labels":[],"label_agreement":null},{"id":"W3033515169","doi":"10.3847/1538-4357/abe530","title":"On the Color–Metallicity Relation of the Red Clump and the Reddening toward the Magellanic Clouds","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Istituto Nazionale di Fisica Nucleare; Universidad Nacional Autónoma de México; Max-Planck-Institut für Astrophysik; Nuclear Safety and Security Commission; Ministerio de Economía y Competitividad; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Red clump; Cepheid variable; Large Magellanic Cloud; RR Lyrae variable; Cosmic distance ladder; Extinction (optical mineralogy); Stars; Metallicity","score_opus":0.012868441754041178,"score_gpt":0.21332326030537968,"score_spread":0.2004548185513385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3033515169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941409,0.00022402752,0.0013462909,0.00011917612,0.000010572077,0.000008015353,0.00015203834,0.00003123987,0.003967731],"genre_scores_gemma":[0.9993563,0.00003086198,0.00029875265,0.000024054183,0.00001113832,0.0000018764302,0.000079128586,0.0000058147643,0.00019199909],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963176,0.00012384742,0.000020888712,0.000099589575,0.000080241574,0.000043785305],"domain_scores_gemma":[0.9890694,0.0054361913,0.0028658272,0.000649092,0.0012631046,0.00071639667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012890833,0.0002283257,0.00014425463,0.0017048125,0.00026598494,0.00073553855,0.00043790467,0.0004617597,0.0025234448],"category_scores_gemma":[0.008948541,0.00015906684,0.00017575329,0.0008035157,0.00074418244,0.00036033973,0.0004558909,0.00050089654,0.00045839304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009533982,0.000030230543,0.99287343,0.000006798153,0.000027432088,0.00006514291,0.00008529979,0.0009554175,0.0014362808,0.0006795149,0.00020035217,0.0035447255],"study_design_scores_gemma":[0.0000058993874,0.000044119675,0.99540895,0.0000074898835,0.000013797619,0.000095704614,0.00010832195,0.0030330427,0.00048283784,0.0005046666,0.00029069072,0.000004462631],"about_ca_topic_score_codex":0.007427652,"about_ca_topic_score_gemma":0.0049727615,"teacher_disagreement_score":0.007427652,"about_ca_system_score_codex":0.00035555148,"about_ca_system_score_gemma":0.00016819939,"threshold_uncertainty_score":0.014768839},"labels":[],"label_agreement":null},{"id":"W3033548758","doi":"10.3847/1538-4357/ab94bb","title":"Erratum: “Detection of Coherent Emission from the Bp Star HD 142990 at uGMRT Frequencies” (2019, ApJ, 877, 123)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Astrophysics; Astronomy; Star (game theory)","score_opus":0.01335035572557514,"score_gpt":0.2174790725133775,"score_spread":0.20412871678780237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3033548758","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.001409588,0.0011225159,0.00038602424,0.05528416,0.90686476,0.00003772077,0.0047904877,0.00056133873,0.029543458],"genre_scores_gemma":[0.02072095,0.0038501031,0.0031262212,0.11489007,0.15705779,0.00009978601,0.012489809,0.0013760674,0.6863892],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9989629,0.000071558825,0.00016423197,0.00017413797,0.0005145574,0.00011265345],"domain_scores_gemma":[0.9947231,0.00084577,0.000380245,0.00038012062,0.0031012206,0.0005695087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010605439,0.0015979998,0.0009785934,0.0030134604,0.0046307375,0.0025956884,0.0016913667,0.0041282224,0.057556618],"category_scores_gemma":[0.0081035625,0.00072691933,0.00088745524,0.0013508976,0.00119867,0.0018144206,0.001267932,0.0045242095,0.043268517],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004720724,0.000014322758,0.0001896738,0.000049196864,0.000006091939,0.0002900563,0.000012540935,0.00002109455,0.0002129225,0.00027219026,0.9954053,0.0034793501],"study_design_scores_gemma":[0.000041740786,0.000045745284,0.0068677077,0.00016563271,0.00003707669,0.00051461335,0.00012170483,0.00014954893,0.0010610112,0.0009192607,0.99002725,0.00004866691],"about_ca_topic_score_codex":0.026880356,"about_ca_topic_score_gemma":0.044578493,"teacher_disagreement_score":0.057556618,"about_ca_system_score_codex":0.0024082486,"about_ca_system_score_gemma":0.0032377862,"threshold_uncertainty_score":0.19254607},"labels":[],"label_agreement":null},{"id":"W3033617754","doi":"10.3847/1538-4357/ab9a54","title":"Dual-wavelength ALMA Observations of Dust Rings in Protoplanetary Disks","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; East Asian Core Observatories Association; Bundesministerium für Bildung und Forschung; Alexander von Humboldt-Stiftung; National Astronomical Observatory of Japan; Koninklijke Nederlandse Akademie van Wetenschappen; European Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Natural Science Foundation of China; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Millimeter; Protoplanetary disk; Submillimeter Array; Planet; Spectral index; Wavelength; Circumstellar dust; Flux (metallurgy); Maxima","score_opus":0.0317586911749766,"score_gpt":0.24106536182788144,"score_spread":0.20930667065290484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3033617754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99794644,0.00008730113,0.0003952069,0.000022186005,0.0000066526795,0.0000039834185,0.0003032637,0.000052902305,0.0011819837],"genre_scores_gemma":[0.9981775,0.00002186194,0.0010871043,0.000015875865,0.000014675537,0.000005634882,0.00039629944,0.0000065814834,0.0002745691],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992335,0.000006816162,0.000002930376,0.000025406394,0.000024553294,0.000016907095],"domain_scores_gemma":[0.99979347,0.000023876837,0.000051146126,0.000030627813,0.000040561485,0.000060414193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015622067,0.00014002141,0.00014630749,0.0006525789,0.0002807327,0.00033688775,0.0002783596,0.00021298703,0.0006377505],"category_scores_gemma":[0.0002701297,0.00015913465,0.00018658534,0.00021807026,0.000088499335,0.00019017725,0.00027033375,0.00021607877,0.0001822564],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010930051,0.00024769665,0.56781316,0.00008055156,0.00017023455,0.00055358507,0.0005662981,0.001137268,0.4018459,0.000490634,0.0012057637,0.024795864],"study_design_scores_gemma":[0.000032866123,0.00008263369,0.99007845,0.0000056161816,0.00003155894,0.00017227614,0.000078603734,0.002896978,0.0052400497,0.00009343687,0.001280258,0.000007268738],"about_ca_topic_score_codex":0.0015228086,"about_ca_topic_score_gemma":0.003527201,"teacher_disagreement_score":0.0015228086,"about_ca_system_score_codex":0.00024806565,"about_ca_system_score_gemma":0.000058332414,"threshold_uncertainty_score":0.0030278563},"labels":[],"label_agreement":null},{"id":"W3033943843","doi":"10.3847/1538-4357/ab8f93","title":"Efficient Methanol Production on the Dark Side of a Prestellar Core","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Jet Propulsion Laboratory; Ural Federal University; Russian Science Foundation; National Astronomical Observatory of Japan; National Radio Astronomy Observatory; Academy of Finland; National Institutes of Natural Sciences; California Institute of Technology; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Methanol; Physics; Carbon monoxide; Astrophysics; Photodissociation; Molecular cloud; Chemistry; Photochemistry; Stars; Catalysis","score_opus":0.02663554804068854,"score_gpt":0.24693207235326134,"score_spread":0.2202965243125728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3033943843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99850607,0.00004816846,0.00017330403,0.000018959689,0.000001547689,0.0000016779702,0.00010012798,0.000021829546,0.0011283746],"genre_scores_gemma":[0.9995617,0.000012424716,0.00011599607,0.000008834414,0.0000017730268,0.0000011625642,0.00010100977,0.0000030666022,0.00019393441],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999726,0.0000011534554,8.4756465e-7,0.000007847603,0.000006485728,0.00001118692],"domain_scores_gemma":[0.9999447,0.0000050967137,0.00001560371,0.000006381163,0.0000071343466,0.000021034586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000034586592,0.00012935906,0.00016264396,0.0002854605,0.00023084717,0.00028126367,0.00018817671,0.00013352718,0.0017032146],"category_scores_gemma":[0.00006486027,0.00012372353,0.00007677183,0.00014343578,0.00018414485,0.00015063504,0.0002941649,0.00015616257,0.00016908122],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004238628,0.0000479261,0.09270691,0.00005703917,0.000044380147,0.00048188397,0.0001762843,0.001259628,0.89782315,0.00047029057,0.00034683436,0.006161735],"study_design_scores_gemma":[0.000024519804,0.0000772458,0.9089768,0.0000053953395,0.000016204871,0.00020351559,0.00014034215,0.003903274,0.08521411,0.00022631904,0.0012042328,0.000008099603],"about_ca_topic_score_codex":0.0025498378,"about_ca_topic_score_gemma":0.0025558893,"teacher_disagreement_score":0.0025498378,"about_ca_system_score_codex":0.00029758827,"about_ca_system_score_gemma":0.000096622505,"threshold_uncertainty_score":0.005697787},"labels":[],"label_agreement":null},{"id":"W3034184139","doi":"10.3847/1538-4357/abbda5","title":"Stars Stripped in Binaries: The Living Gravitational-wave Sources","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Gravitational wave; Astronomy; Astrophysics; Stars; Binary star","score_opus":0.023133516823805062,"score_gpt":0.2941262502307487,"score_spread":0.27099273340694363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3034184139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98771673,0.000060001235,0.009819695,0.00006748192,0.0000066907396,0.000016211483,0.00025829836,0.00018712899,0.0018677189],"genre_scores_gemma":[0.9966216,0.000028084658,0.002251627,0.00001660247,0.0000035134508,0.000007736328,0.00039374534,0.00003578054,0.0006413107],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989593,0.000028093427,0.00000584743,0.000018957422,0.00002659921,0.000024606325],"domain_scores_gemma":[0.99934167,0.0003305064,0.00008380053,0.00006909975,0.000064885724,0.00011008619],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048248903,0.0002725085,0.00030118867,0.00044780262,0.00062597846,0.000733331,0.00052799855,0.00050907815,0.0021267151],"category_scores_gemma":[0.0018592486,0.00029912512,0.00038786416,0.00045658156,0.00035804356,0.00065816496,0.00043091722,0.00021757181,0.0004074517],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001524704,0.000083771636,0.1682361,0.000025500565,0.000048278358,0.0003227651,0.000083649255,0.81705076,0.0020514114,0.0047279596,0.00050102355,0.0067162616],"study_design_scores_gemma":[0.000023089247,0.000025523172,0.016388219,0.000005197427,0.000011734664,0.00007311943,0.000022858847,0.9793799,0.0015869448,0.0021321943,0.00033992948,0.000011245248],"about_ca_topic_score_codex":0.013643155,"about_ca_topic_score_gemma":0.009984758,"teacher_disagreement_score":0.013643155,"about_ca_system_score_codex":0.00078778306,"about_ca_system_score_gemma":0.00047299714,"threshold_uncertainty_score":0.027127445},"labels":[],"label_agreement":null},{"id":"W3034369219","doi":"10.3847/1538-4357/abb5f6","title":"The Milky Way’s Shell Structure Reveals the Time of a Radial Collision","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Milky Way; LAMOST; Galaxy; Stars; Galaxy formation and evolution; Dwarf galaxy; Virial mass; Substructure","score_opus":0.008313842752007899,"score_gpt":0.21343515704720567,"score_spread":0.20512131429519778,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3034369219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995492,0.00002292471,0.00013154972,0.000013225233,9.771946e-7,0.0000011574057,0.000031285635,0.000011200745,0.00023838121],"genre_scores_gemma":[0.9996443,0.000009765949,0.00016796315,0.000005726609,7.731202e-7,0.0000014161474,0.000089295885,0.0000087110175,0.000072048366],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991834,0.000016043105,0.0000038975822,0.000020698393,0.000015761741,0.000025202402],"domain_scores_gemma":[0.99965286,0.000093821305,0.00009862431,0.000035821256,0.000039810864,0.00007896388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032481094,0.00017581598,0.0002774344,0.00041203032,0.00040204576,0.00068761327,0.00047139535,0.0003583073,0.00080811785],"category_scores_gemma":[0.001280654,0.0002504469,0.0005393778,0.00027971185,0.0003162656,0.00040166592,0.0006725262,0.00027918324,0.00013203279],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003993994,0.0001453874,0.80752,0.000046972393,0.00042375905,0.000693882,0.00063250476,0.15380545,0.026482102,0.0022866377,0.0006759443,0.0068879183],"study_design_scores_gemma":[0.000077782366,0.00030010406,0.6671697,0.00002058056,0.00015381169,0.00026424942,0.0005834558,0.32525742,0.0040085777,0.0007255707,0.001397157,0.00004163486],"about_ca_topic_score_codex":0.01622037,"about_ca_topic_score_gemma":0.013676498,"teacher_disagreement_score":0.01622037,"about_ca_system_score_codex":0.0007481196,"about_ca_system_score_gemma":0.0003478689,"threshold_uncertainty_score":0.032251894},"labels":[],"label_agreement":null},{"id":"W3034570506","doi":"10.3847/1538-4357/ab8eab","title":"A New Multitracer Approach to Defining the Spiral Arm Width in the Milky Way","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Milky Way; Shock front; Spiral galaxy; Astrophysics; RADIUS; Maser; Shock wave; Density wave theory; Astronomy; Galaxy; Mechanics","score_opus":0.02186725492022988,"score_gpt":0.2454191446367769,"score_spread":0.223551889716547,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3034570506","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8587215,0.0019082815,0.13128752,0.000120900986,0.00002264183,0.000024285555,0.0006000759,0.0002866756,0.0070281397],"genre_scores_gemma":[0.966145,0.0002736297,0.032175492,0.000033575936,0.000036145466,0.00004408131,0.00031455053,0.00007129696,0.0009061773],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99965394,0.000073508236,0.000029735436,0.000110117646,0.00007945415,0.000053204792],"domain_scores_gemma":[0.9982527,0.0005362243,0.0006566305,0.00026162257,0.00020321863,0.00008959848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00092747196,0.00040741503,0.0003084051,0.005778074,0.00028796686,0.0016732574,0.00089308474,0.00042315846,0.0013433696],"category_scores_gemma":[0.0031547213,0.00025281435,0.0006487707,0.002189919,0.0005674433,0.0013585207,0.0013262939,0.00051079417,0.00024039771],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006671907,0.0001594542,0.4998642,0.00035534875,0.00089541764,0.0008824969,0.0011367298,0.11334371,0.11474414,0.05797714,0.0008255143,0.20914868],"study_design_scores_gemma":[0.0000535642,0.00033630553,0.61010283,0.00011404819,0.00037404773,0.0018816562,0.0007744567,0.30066812,0.027869018,0.04308764,0.014558673,0.0001797297],"about_ca_topic_score_codex":0.0015282822,"about_ca_topic_score_gemma":0.0018475113,"teacher_disagreement_score":0.005778074,"about_ca_system_score_codex":0.0005520694,"about_ca_system_score_gemma":0.000217504,"threshold_uncertainty_score":0.004905045},"labels":[],"label_agreement":null},{"id":"W3034657818","doi":"10.3847/1538-4357/abb36d","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: How Broad Emission Line Widths Change When Luminosity Changes","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"National Key Research and Development Program of China; Science and Technology Facilities Council; National Natural Science Foundation of China","keywords":"Reverberation mapping; Quasar; Luminosity; Sky; Line (geometry); Virial theorem; Photoionization; Emission spectrum","score_opus":0.03697845919005515,"score_gpt":0.23317135892731153,"score_spread":0.19619289973725637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3034657818","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933321,0.000096832744,0.0006112598,0.000078956415,0.0000046334153,0.000004972626,0.004795894,0.000060163013,0.0010151329],"genre_scores_gemma":[0.9904757,0.000050684637,0.00072103686,0.000025014166,0.000005294658,0.000006883108,0.008369328,0.000034184966,0.00031185232],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995763,0.00012796884,0.000019663643,0.0001161658,0.00009247459,0.0000674153],"domain_scores_gemma":[0.9979291,0.00036628504,0.0006991432,0.00030896105,0.00044452352,0.0002519823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009643009,0.00016629403,0.00012538413,0.00086432486,0.00016448727,0.00052279857,0.0002400203,0.00019184462,0.0005904864],"category_scores_gemma":[0.0022324708,0.00009292981,0.00013600574,0.0010081332,0.00016270646,0.00035897113,0.0004790307,0.00017886706,0.00030258775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001018666,0.000027584534,0.97592205,0.000024355804,0.00009011439,0.000043118143,0.0003586185,0.001653764,0.0021963029,0.00014858299,0.0031884252,0.016245175],"study_design_scores_gemma":[9.592839e-7,0.000005637976,0.9982199,0.000002307912,0.0000042681518,0.000013277089,0.000062952786,0.00095587445,0.00018607291,0.000022491418,0.00052369054,0.000002472864],"about_ca_topic_score_codex":0.02097695,"about_ca_topic_score_gemma":0.030673478,"teacher_disagreement_score":0.02097695,"about_ca_system_score_codex":0.00022823885,"about_ca_system_score_gemma":0.00013640679,"threshold_uncertainty_score":0.04170972},"labels":[],"label_agreement":null},{"id":"W3034856229","doi":"10.3847/1538-4357/ab9c9b","title":"Mid-infrared Studies of HD 113766 and HD 172555: Assessing Variability in the Terrestrial Zone of Young Exoplanetary Systems","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Astronomy; Infrared; Population; Infrared excess; Meteoroid; Photometry (optics); Planetesimal; Planet; Stars","score_opus":0.03357737122965334,"score_gpt":0.2649579347120769,"score_spread":0.23138056348242356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3034856229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99949086,0.000057503414,0.000045534514,0.000003841563,9.082301e-7,0.0000020094199,0.00009043443,0.000002287246,0.00030662215],"genre_scores_gemma":[0.9995466,0.000026443471,0.00009652071,0.000005860156,0.0000026169675,0.0000019628221,0.00020987759,0.000001409601,0.0001087636],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999001,0.000009340731,0.0000071254412,0.000026656178,0.000028227367,0.00002852885],"domain_scores_gemma":[0.99973935,0.000028853727,0.00009173072,0.000014901062,0.000038327587,0.00008677952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021459431,0.0001948438,0.00019183091,0.0011439251,0.0005323409,0.0004549458,0.00020153055,0.00018661487,0.0006517128],"category_scores_gemma":[0.00034424188,0.00010189815,0.00014900889,0.0006341279,0.00025606525,0.0002649912,0.00043277605,0.00019801705,0.00017158758],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012614492,0.000041840594,0.94899905,0.000015953168,0.000031667238,0.00021976054,0.00047730855,0.00016063602,0.0463453,0.00004949082,0.00006502059,0.0034678113],"study_design_scores_gemma":[7.851312e-7,0.000010260692,0.99926406,7.2971386e-7,0.0000017680283,0.000055016855,0.00008060813,0.000039579565,0.0004732769,0.0000028718357,0.00007018058,8.683882e-7],"about_ca_topic_score_codex":0.0072022015,"about_ca_topic_score_gemma":0.014045853,"teacher_disagreement_score":0.0072022015,"about_ca_system_score_codex":0.0003689241,"about_ca_system_score_gemma":0.000095710166,"threshold_uncertainty_score":0.014320552},"labels":[],"label_agreement":null},{"id":"W3034918350","doi":"10.3847/1538-4357/ab952f","title":"The Copula of the Cosmological Matter Density Field is Non-Gaussian","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Copula (linguistics); Logarithm; Gaussian; Residual; Cosmology; Dark matter","score_opus":0.008077836196102094,"score_gpt":0.20744114058662158,"score_spread":0.1993633043905195,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3034918350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.53858656,0.0003670234,0.45129964,0.0010779297,0.00007122588,0.00004646108,0.0002702003,0.0005749916,0.0077059604],"genre_scores_gemma":[0.9907176,0.0001573725,0.0074559953,0.00009530926,0.00002990043,0.00001678459,0.0001118635,0.00007022786,0.0013448972],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99944085,0.00020941834,0.000015971922,0.00014688628,0.00007798764,0.00010884786],"domain_scores_gemma":[0.9952792,0.002694833,0.00065583753,0.00066002517,0.00044929926,0.00026082588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017248095,0.00044985072,0.000631026,0.0006422315,0.0005481544,0.0014367227,0.0007511278,0.00056300225,0.00243742],"category_scores_gemma":[0.01200028,0.00042114712,0.0006536044,0.000632443,0.0020532913,0.002054766,0.0006869671,0.0009950451,0.00033756724],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012081432,0.000063780564,0.017486567,0.00014336115,0.00021458918,0.00073696795,0.0003818089,0.6637769,0.0065412275,0.29408982,0.0040549943,0.0123891365],"study_design_scores_gemma":[0.0000100383895,0.000029330302,0.009115672,0.000016650276,0.00001786307,0.00011559257,0.00006186889,0.93183273,0.00090640184,0.05727698,0.00057963707,0.000037205347],"about_ca_topic_score_codex":0.0105891125,"about_ca_topic_score_gemma":0.004568028,"teacher_disagreement_score":0.0105891125,"about_ca_system_score_codex":0.00085688394,"about_ca_system_score_gemma":0.00074517634,"threshold_uncertainty_score":0.021054983},"labels":[],"label_agreement":null},{"id":"W3035017618","doi":"10.3847/1538-4357/ab9198","title":"Survey of Extremely High-velocity Outflows in Sloan Digital Sky Survey Quasars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Western University; York University; University of Toronto","funders":"","keywords":"Quasar; Sky; Spectral line; Emission spectrum; Black hole (networking); Absorption (acoustics); Luminosity; Line (geometry)","score_opus":0.02484214914591631,"score_gpt":0.22614396780256626,"score_spread":0.20130181865664995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3035017618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971264,0.00016196906,0.00014721147,0.00001971276,0.000001939627,0.000007097318,0.0017729757,0.000020826345,0.0007420224],"genre_scores_gemma":[0.99521834,0.00015620334,0.00025992052,0.000024719273,0.000006222961,0.000008133264,0.0039393483,0.00000497881,0.00038217576],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997248,0.000035823454,0.00002711107,0.000052743366,0.00007955448,0.0000799634],"domain_scores_gemma":[0.99842787,0.00013062799,0.00068489154,0.00008301352,0.00023100866,0.00044270052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043330173,0.0002109979,0.00017513164,0.0033965656,0.00031659595,0.0005534727,0.00016684452,0.0001366423,0.0009939196],"category_scores_gemma":[0.000661339,0.00012002255,0.00019458795,0.0018373295,0.00023310851,0.00027377022,0.0006671803,0.00015542931,0.00021640082],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002203002,0.000013188844,0.99492234,0.000019983125,0.000028896919,0.00006156134,0.00008698031,0.000051389157,0.0011777594,0.000041581494,0.00036728434,0.0032070293],"study_design_scores_gemma":[0.0000011515828,0.000007926961,0.9991416,0.0000037618768,0.000005310761,0.000042712392,0.00007487606,0.00006241808,0.00010223165,0.000007791074,0.00054869434,0.0000014511116],"about_ca_topic_score_codex":0.011757592,"about_ca_topic_score_gemma":0.01937841,"teacher_disagreement_score":0.011757592,"about_ca_system_score_codex":0.00030686354,"about_ca_system_score_gemma":0.00026233235,"threshold_uncertainty_score":0.023378313},"labels":[],"label_agreement":null},{"id":"W3035186706","doi":"10.3847/1538-4357/ab9b24","title":"Atmospheric Temperature Inversions and He i 5876 Core Profile Structure in White Dwarfs","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Los Alamos National Laboratory; Laboratory Directed Research and Development; National Aeronautics and Space Administration; National Science Foundation","keywords":"Astrophysics; Stars; Atmosphere (unit); Physics; Opacity; White dwarf; Line (geometry); Effective temperature; Hydrogen; Spectral line; Atmospheric temperature; Astronomy; Atmospheric sciences; Optics; Meteorology","score_opus":0.009394738738615228,"score_gpt":0.2065625097725758,"score_spread":0.19716777103396055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3035186706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99949574,0.000020691718,0.00021112898,0.0000018080152,5.1180564e-7,5.3475117e-7,0.000055916626,0.000011470419,0.00020222836],"genre_scores_gemma":[0.99979895,0.0000055482246,0.00007321328,7.135086e-7,4.4336738e-7,2.9607338e-7,0.00008093374,0.0000022244228,0.00003768661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994016,0.0000053219546,0.000003837518,0.000024815197,0.000015597852,0.000010294529],"domain_scores_gemma":[0.99981683,0.000027554572,0.00007096973,0.000021405764,0.000028967661,0.00003435526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011080342,0.0001419397,0.00014374357,0.00036547155,0.00016139814,0.0003141584,0.00014247952,0.00014354633,0.00048571758],"category_scores_gemma":[0.00036147097,0.000099208904,0.00012507044,0.00022322431,0.00016770998,0.00021024841,0.00022508131,0.0000884741,0.00013736957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016945883,0.000029331633,0.9062378,0.000018721968,0.000043929653,0.000120369725,0.00014933554,0.003030821,0.0841648,0.00014921736,0.0000697395,0.005816502],"study_design_scores_gemma":[0.0000027511933,0.000029144443,0.98775476,0.000001905845,0.000010271929,0.00010065891,0.000059422408,0.0049492097,0.006787275,0.00008971848,0.00021102242,0.000003902902],"about_ca_topic_score_codex":0.0030617076,"about_ca_topic_score_gemma":0.0033433756,"teacher_disagreement_score":0.0030617076,"about_ca_system_score_codex":0.00022914985,"about_ca_system_score_gemma":0.000068677415,"threshold_uncertainty_score":0.00608778},"labels":[],"label_agreement":null},{"id":"W3035655882","doi":"10.1086/522567","title":"The White Dwarf Cooling Sequence of NGC 6397","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":183,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia","funders":"","keywords":"Physics; Astrophysics; White dwarf; Globular cluster; Luminosity function; Distance modulus; Astronomy; Context (archaeology); Open cluster; Star cluster; Redshift; Luminosity; Galaxy; Apparent magnitude; Star count; Stars; T Tauri star","score_opus":0.010871167296565124,"score_gpt":0.23515537028364578,"score_spread":0.22428420298708066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3035655882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986682,0.000031099007,0.00012415841,0.000007801714,0.0000015595335,0.0000021077399,0.0003626218,0.00001376443,0.0007886591],"genre_scores_gemma":[0.9976908,0.000035352026,0.00022229293,0.000007097943,0.0000028404027,0.0000045024603,0.0016243776,0.000010577821,0.0004021067],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999311,0.0000041837266,0.0000035020978,0.000017619222,0.00002405847,0.000019579069],"domain_scores_gemma":[0.99972254,0.00004163081,0.0000710151,0.00004378782,0.000051392435,0.00006966313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001396707,0.00014344536,0.00022293291,0.0007442839,0.00048380293,0.0003578939,0.00019208551,0.00016985167,0.0008852042],"category_scores_gemma":[0.00043675117,0.00007502845,0.00022504805,0.00084092066,0.00021913658,0.000086321495,0.00030408,0.00018520773,0.00029366752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047302607,0.00006324367,0.8721612,0.00006828183,0.00007851198,0.002202453,0.0019483049,0.0037923914,0.090799384,0.0011266363,0.0013397338,0.025946787],"study_design_scores_gemma":[0.000005724227,0.000036930887,0.9950832,0.0000058439277,0.000010679129,0.00034870673,0.00010934489,0.0009020369,0.0021893987,0.00016277323,0.0011394385,0.000005842819],"about_ca_topic_score_codex":0.023364307,"about_ca_topic_score_gemma":0.03075356,"teacher_disagreement_score":0.023364307,"about_ca_system_score_codex":0.0005424685,"about_ca_system_score_gemma":0.00038495337,"threshold_uncertainty_score":0.046456635},"labels":[],"label_agreement":null},{"id":"W3035662846","doi":"10.3847/1538-4357/abc01c","title":"JWST Transit Spectra. I. Exploring Potential Biases and Opportunities in Retrievals of Tidally Locked Hot Jupiters with Clouds and Hazes","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Aeronautics and Space Administration","keywords":"Exoplanet; Transit (satellite); Spectral line; Hot Jupiter; Planet; Metallicity; Atmospheric models; Atmospheric model","score_opus":0.05649999035691497,"score_gpt":0.22239764652853322,"score_spread":0.16589765617161825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3035662846","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98979414,0.00006791974,0.007649943,0.000049128146,0.0000093968965,0.000012924776,0.00077414466,0.000606674,0.0010357758],"genre_scores_gemma":[0.9932916,0.00001829372,0.0055030975,0.000011859804,0.000004472346,0.0000045230067,0.00084377924,0.00012940059,0.00019294278],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984264,0.000020894731,0.000014159714,0.00006104365,0.000038486454,0.000022702356],"domain_scores_gemma":[0.99949276,0.00014882542,0.00008555002,0.00013750116,0.0000990055,0.000036286183],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050635106,0.00028442385,0.00019083593,0.00067837565,0.00032860806,0.0005349444,0.0005169715,0.00031854786,0.0008622261],"category_scores_gemma":[0.0021007624,0.00022543204,0.00044040932,0.00075347774,0.00023269014,0.0010184229,0.00038003,0.0002877602,0.0002135782],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015526194,0.00019657022,0.4784166,0.00022093765,0.00059172546,0.00051494205,0.0007476652,0.26708782,0.15568548,0.0030392637,0.0023091608,0.08963722],"study_design_scores_gemma":[0.00016723372,0.000120654324,0.23147754,0.000021389671,0.0001054386,0.00024281899,0.00023861347,0.70912194,0.05414601,0.0015519406,0.0027532992,0.00005307006],"about_ca_topic_score_codex":0.011720372,"about_ca_topic_score_gemma":0.014121764,"teacher_disagreement_score":0.011720372,"about_ca_system_score_codex":0.00039863185,"about_ca_system_score_gemma":0.00027582952,"threshold_uncertainty_score":0.023304284},"labels":[],"label_agreement":null},{"id":"W3036416766","doi":"10.3847/1538-4357/ab9107","title":"Hot Plasma Effects on the Pitch-angle Scattering Rates of Radiation Belt Electrons Due to Plasmaspheric Hiss","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Memorial University of Newfoundland","funders":"National Natural Science Foundation of China","keywords":"Hiss; Physics; Electron; Pitch angle; Van Allen radiation belt; Atomic physics; Scattering; Plasma; Diffusion; Electron scattering; Computational physics; Nuclear physics; Optics; Geophysics; Magnetosphere","score_opus":0.006612192633171097,"score_gpt":0.21051161371711186,"score_spread":0.20389942108394077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3036416766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995174,0.0002492583,0.0024442247,0.0000321415,0.0000100299385,0.000005812921,0.00009264264,0.00005481388,0.0019370373],"genre_scores_gemma":[0.9996847,0.000054010252,0.000093939525,0.0000027318085,0.0000024320436,0.0000010510087,0.000034073455,0.0000066039674,0.00012063903],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999293,0.000014152962,0.0000039166807,0.000017007347,0.000016613925,0.000019059318],"domain_scores_gemma":[0.99961877,0.00017502859,0.000071919596,0.000035758254,0.00006196375,0.000036526588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028429236,0.0004176855,0.00019495955,0.00038571339,0.00020484765,0.00032646753,0.000251987,0.00016931418,0.0012783793],"category_scores_gemma":[0.0009433797,0.00016049929,0.0002881671,0.00027921467,0.00031920298,0.00047776435,0.000409937,0.00023696962,0.00010463174],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002140427,0.00015107189,0.22199832,0.00045463623,0.00037586896,0.0024877503,0.00097194436,0.3301992,0.39706174,0.011745469,0.00083624944,0.031577367],"study_design_scores_gemma":[0.00011994499,0.00032131653,0.2055534,0.000036524543,0.00013310232,0.00055581273,0.0003962942,0.67421347,0.113671914,0.0034594531,0.0014525169,0.000086225875],"about_ca_topic_score_codex":0.0017049003,"about_ca_topic_score_gemma":0.00059329154,"teacher_disagreement_score":0.0017049003,"about_ca_system_score_codex":0.00030077918,"about_ca_system_score_gemma":0.00008605759,"threshold_uncertainty_score":0.0042765737},"labels":[],"label_agreement":null},{"id":"W3036999981","doi":"10.3847/1538-4357/ab9f9d","title":"The Effect of Misalignment between the Rotation Axis and Magnetic Field on the Circumstellar Disk","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Outflow; Physics; Protostar; Rotation (mathematics); Astrophysics; Magnetic field; Magnetohydrodynamic drive; Circumstellar disk; Magnetohydrodynamics; Bipolar outflow; Thermal; Star formation; Stars; Geometry; Meteorology","score_opus":0.007905538172101894,"score_gpt":0.22181083817106476,"score_spread":0.21390529999896285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3036999981","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991615,0.000024691384,0.00026160094,0.000022360224,0.0000033431995,0.0000030886622,0.00003562548,0.000015439366,0.00047242295],"genre_scores_gemma":[0.9997646,0.000013406072,0.00012881427,0.000004590796,0.0000011054685,0.0000019707895,0.000025781239,0.0000042556717,0.00005557738],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998753,0.00004381022,0.000006711867,0.00001756261,0.000016665632,0.00003995659],"domain_scores_gemma":[0.99914515,0.00042561063,0.00015673236,0.00006180123,0.000045391193,0.00016534152],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033917968,0.00036183815,0.00035215952,0.00022146346,0.0004828286,0.0007860197,0.00048516417,0.00046794632,0.0010366075],"category_scores_gemma":[0.002035681,0.00023945708,0.00041573407,0.00020197705,0.00057464873,0.00037057663,0.00039087803,0.0004508456,0.000112879585],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00060124556,0.00015718245,0.054053802,0.000040627674,0.00010044204,0.00047936093,0.000077208366,0.9228393,0.018628707,0.0011369191,0.00018667195,0.0016984871],"study_design_scores_gemma":[0.00019964513,0.00070452807,0.033712618,0.000016115962,0.00007338849,0.00013936851,0.00014301861,0.9542135,0.010004663,0.00041951006,0.00034455603,0.000028991555],"about_ca_topic_score_codex":0.0080063,"about_ca_topic_score_gemma":0.0037706438,"teacher_disagreement_score":0.0080063,"about_ca_system_score_codex":0.00075833505,"about_ca_system_score_gemma":0.00044254868,"threshold_uncertainty_score":0.015919387},"labels":[],"label_agreement":null},{"id":"W3037048429","doi":"10.3847/1538-4357/aba0b2","title":"The Massive and Distant Clusters of WISE Survey. IX. High Radio Activity in a Merging Cluster","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Grantová Agentura České Republiky","keywords":"Galaxy cluster; Radio galaxy; Jansky; X-shaped radio galaxy; Cluster (spacecraft); Brightest cluster galaxy; Population; Galaxy","score_opus":0.008739039423009938,"score_gpt":0.20922763925178745,"score_spread":0.2004885998287775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037048429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99926585,0.00007922804,0.000040230618,0.000025118816,0.0000014761978,0.0000020262348,0.00010146824,0.000004563683,0.0004800683],"genre_scores_gemma":[0.99895775,0.00004773522,0.00021201647,0.00001842211,0.000009061166,0.0000019622366,0.00051472493,0.00000252468,0.00023577153],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984944,0.000014067166,0.000009957958,0.000044591718,0.000042352352,0.000039576174],"domain_scores_gemma":[0.9995303,0.000025591227,0.00020292506,0.00002861916,0.000043200747,0.00016938004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015578036,0.00016905398,0.00025479475,0.0014338414,0.0006465935,0.00052977883,0.0002169878,0.00020225822,0.0010302376],"category_scores_gemma":[0.00040423384,0.00011620532,0.000165755,0.0011070516,0.0002930723,0.0003383318,0.0008342115,0.00020000678,0.00025149688],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008291884,0.000018751145,0.9862968,0.000013114752,0.000023967417,0.00014964317,0.00062656094,0.00007002586,0.0076951617,0.00019199177,0.00037756545,0.004453556],"study_design_scores_gemma":[8.8207975e-7,0.000011275019,0.99924076,0.0000013085919,0.00000449625,0.00007567896,0.00016600864,0.000053577183,0.00014743488,0.0000121813,0.00028501925,0.0000012805698],"about_ca_topic_score_codex":0.0071598934,"about_ca_topic_score_gemma":0.018198034,"teacher_disagreement_score":0.0071598934,"about_ca_system_score_codex":0.00028026386,"about_ca_system_score_gemma":0.00017377066,"threshold_uncertainty_score":0.01423645},"labels":[],"label_agreement":null},{"id":"W3037219258","doi":"10.3847/1538-4357/abb599","title":"The Complete Redshift Distribution of Dusty Star-forming Galaxies from the SPT-SZ Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":120,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute","keywords":"Physics; Astrophysics; Redshift; Galaxy; Redshift survey; Astronomy; Star (game theory); Star formation; Red shift","score_opus":0.020258629523438022,"score_gpt":0.2191664253690606,"score_spread":0.1989077958456226,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037219258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99682766,0.00009685375,0.0001948898,0.000027827826,0.0000018804564,0.000005229367,0.0019668958,0.000022681003,0.0008560272],"genre_scores_gemma":[0.9941644,0.0001077747,0.00021055952,0.000014291417,0.0000072797025,0.000004909944,0.0051395674,0.000007735328,0.00034341673],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977857,0.000017567645,0.000018870118,0.00005499392,0.000081294274,0.000048813068],"domain_scores_gemma":[0.9993345,0.00005424909,0.00021065591,0.00007255814,0.00013587486,0.00019206943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021397832,0.00021933035,0.00021624097,0.0018554599,0.00022371118,0.00051641255,0.00024201398,0.0001403687,0.0021303238],"category_scores_gemma":[0.0007270291,0.0001192276,0.00022091136,0.001326465,0.00022556899,0.00030368887,0.00073940103,0.00017948211,0.00061636354],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000464113,0.000010856689,0.9865536,0.00001558855,0.000042703934,0.00013898761,0.00020442076,0.00015010367,0.004131595,0.00013377455,0.0006949278,0.007877137],"study_design_scores_gemma":[0.0000014669132,0.000009586444,0.99909925,0.0000015418107,0.0000048026773,0.00010044012,0.000048256356,0.00010981897,0.00019728015,0.00001391328,0.00041269907,9.778918e-7],"about_ca_topic_score_codex":0.0052624894,"about_ca_topic_score_gemma":0.0049151937,"teacher_disagreement_score":0.0052624894,"about_ca_system_score_codex":0.00020533243,"about_ca_system_score_gemma":0.00018357651,"threshold_uncertainty_score":0.010463715},"labels":[],"label_agreement":null},{"id":"W3037653511","doi":"10.3847/1538-4357/ab980c","title":"Erratum: “A Deep Near-infrared [Fe ii]+[Si i] Emission Line Image of the Supernova Remnant Cassiopeia A” (2018, ApJ, 866, 139)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Cassiopeia A; Physics; Supernova remnant; Supernova; Astrophysics; Line (geometry); Infrared; Astronomy","score_opus":0.01267786535656454,"score_gpt":0.23450135255867774,"score_spread":0.2218234872021132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037653511","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0016876688,0.0018294463,0.0003422657,0.058558132,0.90754604,0.000025774145,0.0034489406,0.00042249283,0.026139215],"genre_scores_gemma":[0.022301476,0.008195095,0.0037650208,0.077864856,0.20946579,0.00008174683,0.013851128,0.0017366488,0.66273826],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9995202,0.000032821463,0.00008551182,0.000096088064,0.00020683296,0.000058560097],"domain_scores_gemma":[0.9977672,0.00034721952,0.00019836515,0.00017662202,0.0012027897,0.00030779437],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005898561,0.0013055272,0.00068665034,0.0021470012,0.0028874455,0.0022203666,0.0015422798,0.0030459606,0.053324908],"category_scores_gemma":[0.0063949497,0.0005737842,0.0006906741,0.0011026264,0.0009955894,0.001679462,0.0013521513,0.004058626,0.03365911],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040189276,0.000008795041,0.00020251605,0.00006500051,0.000005272023,0.0004915507,0.000023429615,0.000024866167,0.00016551309,0.00042673503,0.99308395,0.005462193],"study_design_scores_gemma":[0.000016749835,0.000013759955,0.0023661072,0.000127468,0.000016220505,0.0007063328,0.000090568086,0.0000660532,0.00038622966,0.0006738018,0.9955179,0.000018853172],"about_ca_topic_score_codex":0.020447513,"about_ca_topic_score_gemma":0.02753139,"teacher_disagreement_score":0.053324908,"about_ca_system_score_codex":0.0015906466,"about_ca_system_score_gemma":0.0022187077,"threshold_uncertainty_score":0.17838961},"labels":[],"label_agreement":null},{"id":"W3037701043","doi":"10.3847/1538-4357/abd776","title":"Virialization of the Inner CGM in the FIRE Simulations and Implications for Galaxy Disks, Star Formation, and Feedback","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":129,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Flatiron Health; Northwestern University; National Aeronautics and Space Administration; Space Telescope Science Institute; Research Corporation for Science Advancement; National Science Foundation","keywords":"Physics; Virial theorem; Astrophysics; Virial mass; Halo; Galaxy; Galaxy formation and evolution; Redshift; Star formation; RADIUS; Astronomy","score_opus":0.010729035415424063,"score_gpt":0.2352616474175449,"score_spread":0.22453261200212085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037701043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99685836,0.00003615208,0.001204682,0.00011066471,0.000008370576,0.0000074207305,0.00013277424,0.000039749357,0.0016019457],"genre_scores_gemma":[0.9989592,0.0000218198,0.00062081724,0.000031355794,0.0000034854227,0.0000077340455,0.000100644735,0.000020688796,0.0002344132],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998523,0.000043482465,0.000005627975,0.000026330777,0.00002340028,0.000048883383],"domain_scores_gemma":[0.99917525,0.00035954095,0.0001030729,0.0000827035,0.00007051265,0.00020892228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000776724,0.00034465123,0.0005967976,0.00032183825,0.0006852298,0.0012237198,0.0010956664,0.00079683546,0.0011036289],"category_scores_gemma":[0.0034481415,0.00028449515,0.0006039249,0.00025700938,0.00088327687,0.0007178002,0.0007628022,0.0010498206,0.00008478266],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040517355,0.00016856835,0.045991268,0.000032471722,0.00012941567,0.0002748371,0.000263524,0.93540925,0.006317882,0.008166139,0.00042557862,0.0024159097],"study_design_scores_gemma":[0.00008947568,0.00009455871,0.008451371,0.000008597996,0.00002431553,0.00003308432,0.000097817916,0.98799825,0.0017000468,0.0011882357,0.00029563732,0.000018683],"about_ca_topic_score_codex":0.02252527,"about_ca_topic_score_gemma":0.0106200455,"teacher_disagreement_score":0.02252527,"about_ca_system_score_codex":0.0011393749,"about_ca_system_score_gemma":0.0007082482,"threshold_uncertainty_score":0.04478836},"labels":[],"label_agreement":null},{"id":"W3037861462","doi":"10.3847/1538-4357/ab9aba","title":"Multiband GPI Imaging of the HR 4796A Debris Disk","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Western University","funders":"National Aeronautics and Space Administration","keywords":"Scattering; Monte Carlo method; Phase (matter); SPHERES; RADIUS; Mie scattering; Background subtraction; Function (biology)","score_opus":0.010323982077777117,"score_gpt":0.2153695401788743,"score_spread":0.20504555810109718,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3037861462","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99524456,0.00008574299,0.0012512936,0.000048226204,0.0000050610442,0.0000083160185,0.00087412156,0.0002462734,0.0022364412],"genre_scores_gemma":[0.99732345,0.00002774664,0.0017247483,0.000015697256,0.000006204559,0.0000033615356,0.00067442027,0.000027847374,0.00019648342],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998925,0.000012383453,0.000006038322,0.00003482086,0.00003459647,0.000019625233],"domain_scores_gemma":[0.99980575,0.000028436985,0.000040991028,0.000055253066,0.0000247082,0.00004497053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003170753,0.00025301208,0.000195785,0.00077064446,0.00024681623,0.00042913135,0.000313398,0.00025685164,0.0013411185],"category_scores_gemma":[0.00038423217,0.00018898927,0.0002643535,0.00053840084,0.00013528361,0.0002907942,0.00035703002,0.00023592809,0.00038656665],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021039029,0.00033394445,0.34410664,0.00019124184,0.0004635701,0.0022648745,0.0008007543,0.03955797,0.5476021,0.0015190358,0.0025843761,0.05847165],"study_design_scores_gemma":[0.00018394488,0.00033722183,0.84324616,0.000028705545,0.00017187491,0.0010100706,0.00020787962,0.07434771,0.075098075,0.000920724,0.00440294,0.000044713826],"about_ca_topic_score_codex":0.002280096,"about_ca_topic_score_gemma":0.003060315,"teacher_disagreement_score":0.002280096,"about_ca_system_score_codex":0.00040211857,"about_ca_system_score_gemma":0.00011435725,"threshold_uncertainty_score":0.004533708},"labels":[],"label_agreement":null},{"id":"W3038183753","doi":"10.3847/1538-4357/aba1e2","title":"The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Manitoba; McMaster University; Queen's University; Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Japan Society for the Promotion of Science; Canadian Space Agency; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; Universities Space Research Association; National Natural Science Foundation of China; Chinese Academy of Sciences; Academia Sinica","keywords":"Protein filament; Magnetic field; James Clerk Maxwell Telescope; Field (mathematics); Molecular cloud; Magnetic structure; Star formation; Projection (relational algebra)","score_opus":0.014173700959281407,"score_gpt":0.22156834330102945,"score_spread":0.20739464234174804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3038183753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978684,0.000049680057,0.00026940563,0.000030067002,0.0000016074003,0.0000051648226,0.00091342285,0.00007692712,0.00078526785],"genre_scores_gemma":[0.9983925,0.000026632059,0.00038011355,0.000015347172,0.000005857902,0.000005067591,0.0010825401,0.00001148879,0.00008049383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990356,0.0000103337425,0.0000054036896,0.00002541057,0.000030680418,0.000024667059],"domain_scores_gemma":[0.9995733,0.000035247052,0.00018869151,0.00004952098,0.0000462535,0.00010698132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011666742,0.00014959485,0.00017973043,0.0009850829,0.00032631567,0.0003578833,0.0002187043,0.00024247062,0.00083353533],"category_scores_gemma":[0.0003756842,0.00011142835,0.00018414768,0.0009696443,0.0002496673,0.0001973752,0.00036993582,0.00018722922,0.00014766124],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020238338,0.00006605578,0.9202269,0.00004744901,0.00009695118,0.0005123995,0.0002948072,0.002247298,0.06167571,0.00040795986,0.0015545541,0.012667636],"study_design_scores_gemma":[0.0000070515944,0.000010635229,0.9970169,0.0000030362214,0.000009559341,0.00011490245,0.000046365672,0.0016057852,0.00061754073,0.0000448619,0.00051886076,0.0000043692703],"about_ca_topic_score_codex":0.019155225,"about_ca_topic_score_gemma":0.03791541,"teacher_disagreement_score":0.019155225,"about_ca_system_score_codex":0.0005462291,"about_ca_system_score_gemma":0.00022059205,"threshold_uncertainty_score":0.038087487},"labels":[],"label_agreement":null},{"id":"W3038744945","doi":"10.3847/1538-4357/aba4ac","title":"A Distant Fast Radio Burst Associated with Its Host Galaxy by the Very Large Array","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":93,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; Canadian Institute for Advanced Research","funders":"","keywords":"Fast radio burst; Jansky; Galaxy; Photometry (optics); Redshift; Host (biology)","score_opus":0.010409283498251248,"score_gpt":0.2642351059719414,"score_spread":0.2538258224736901,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3038744945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99243224,0.00035771687,0.0030938676,0.00009353484,0.00003301244,0.00001541037,0.0008867495,0.00015026778,0.0029372573],"genre_scores_gemma":[0.996172,0.000051516698,0.0019686562,0.000025636784,0.00003647299,0.0000036643528,0.0007527313,0.000010844277,0.0009785534],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975544,0.000027155658,0.000014693606,0.0000959852,0.000066548535,0.00004019977],"domain_scores_gemma":[0.99914217,0.00015982757,0.00030013177,0.00015931595,0.00008239153,0.000156082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003546689,0.00015453096,0.00016843998,0.00077096367,0.00028003042,0.00060067466,0.00025050875,0.00022999258,0.002070809],"category_scores_gemma":[0.0008137628,0.00011527197,0.000146118,0.00043844935,0.0002242273,0.00030687233,0.0004900839,0.00023718596,0.000414358],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006451372,0.000080660255,0.877111,0.000057456105,0.000100808116,0.0013534203,0.00026421063,0.00071427005,0.06418927,0.0009783843,0.0016716127,0.052833773],"study_design_scores_gemma":[0.000024000396,0.0002076981,0.9806897,0.000013722266,0.000050481474,0.002293795,0.00010705554,0.002787828,0.008554861,0.00042592446,0.0048240465,0.000020770058],"about_ca_topic_score_codex":0.0014876478,"about_ca_topic_score_gemma":0.0028684144,"teacher_disagreement_score":0.002070809,"about_ca_system_score_codex":0.0002846544,"about_ca_system_score_gemma":0.0001038162,"threshold_uncertainty_score":0.00692755},"labels":[],"label_agreement":null},{"id":"W3039097989","doi":"10.3847/1538-4357/abca96","title":"Cycle-StarNet: Bridging the Gap between Theory and Data by Leveraging Large Data Sets","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Spectral line; Synthetic data; Bridging (networking); Residual; Set (abstract data type); Data set; Astronomical spectroscopy; Calibration; Experimental data","score_opus":0.03755557215105797,"score_gpt":0.283821652953197,"score_spread":0.24626608080213902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3039097989","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08684689,0.0011887004,0.7255202,0.0017991592,0.0005085718,0.00055947487,0.015362644,0.16264907,0.0055652494],"genre_scores_gemma":[0.21713598,0.00036892574,0.7250731,0.0007090624,0.00012739074,0.00059578975,0.04530977,0.009199281,0.0014806595],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9961641,0.0014330012,0.0002326329,0.0011432053,0.00087886635,0.00014821497],"domain_scores_gemma":[0.98788106,0.0052457955,0.0005173399,0.0047219475,0.0010335771,0.00060017913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.009649876,0.0015287808,0.0013054922,0.0032353203,0.0008425801,0.002762355,0.004555573,0.0016314066,0.005385505],"category_scores_gemma":[0.03141539,0.001169615,0.0015719922,0.0030971987,0.0016608349,0.005319805,0.0060856333,0.0021978123,0.002590356],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012639544,0.0007267385,0.030038005,0.0012031706,0.0011919998,0.00057670294,0.00088051334,0.39075413,0.00787427,0.03121245,0.09323029,0.44104782],"study_design_scores_gemma":[0.00008476102,0.00007733795,0.0015056955,0.000052868716,0.000025880943,0.00006587995,0.00010570048,0.9482064,0.0031674858,0.02899046,0.017673383,0.000044073655],"about_ca_topic_score_codex":0.0068600443,"about_ca_topic_score_gemma":0.013394267,"teacher_disagreement_score":0.009649876,"about_ca_system_score_codex":0.0013053108,"about_ca_system_score_gemma":0.002312404,"threshold_uncertainty_score":0.051034033},"labels":[],"label_agreement":null},{"id":"W3039111245","doi":"10.3847/1538-4357/abbc6c","title":"JWST Transit Spectra. II. Constraining Aerosol Species, Particle-size Distributions, Temperature, and Metallicity for Cloudy Exoplanets","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Aerosol; James Webb Space Telescope; Metallicity; Transit (satellite); Wavelength; Atmosphere (unit); Exoplanet; Absorption (acoustics)","score_opus":0.020060826094463483,"score_gpt":0.2230714064097518,"score_spread":0.2030105803152883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3039111245","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.991377,0.00012344203,0.0026706348,0.00009001676,0.000010451725,0.000020934862,0.0032823035,0.0005129675,0.0019122979],"genre_scores_gemma":[0.99175864,0.000053143205,0.0034938308,0.000029062061,0.000009042676,0.0000088531815,0.0042452295,0.00015717487,0.00024507171],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998983,0.000010917776,0.000005445055,0.000038143764,0.00002935322,0.000017846909],"domain_scores_gemma":[0.999671,0.000056267636,0.00008760726,0.00008264177,0.00005130683,0.000051143372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046822918,0.000560997,0.00022984832,0.0009214446,0.00051181595,0.0005375292,0.00052170566,0.00048255434,0.0008022139],"category_scores_gemma":[0.001002265,0.00037331058,0.00058754464,0.0007364749,0.0002458739,0.0009550474,0.00045565653,0.0003804637,0.0003568878],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007756543,0.00018248384,0.74240214,0.00022813614,0.00039272106,0.0006645833,0.0003747544,0.108211614,0.1115832,0.0018850064,0.0037107167,0.02958916],"study_design_scores_gemma":[0.00014499453,0.00015609124,0.70254004,0.000042887856,0.00012221785,0.0002676279,0.00019497884,0.26695386,0.022487137,0.0017032787,0.005338361,0.000048530783],"about_ca_topic_score_codex":0.015847845,"about_ca_topic_score_gemma":0.028273912,"teacher_disagreement_score":0.015847845,"about_ca_system_score_codex":0.00062879745,"about_ca_system_score_gemma":0.00033535893,"threshold_uncertainty_score":0.031511188},"labels":[],"label_agreement":null},{"id":"W3039463258","doi":"10.3847/1538-4357/ab9fa3","title":"The Effect of Bars on the Ionized ISM: Optical Emission Lines from Milky Way Analogs","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Notre Dame; Leibniz-Gemeinschaft; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; New Mexico State University; University of Portsmouth; U.S. Department of Energy; Smithsonian Institution; Max-Planck-Institut für Astrophysik; National Science Foundation","keywords":"Physics; Milky Way; Galaxy; Astrophysics; Bar (unit); Ionization; Emission spectrum; Line (geometry); Interstellar medium; Spectral line; Astronomy; Geometry; Ion","score_opus":0.007303755862039896,"score_gpt":0.21251630746581596,"score_spread":0.20521255160377605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3039463258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996315,0.000037442085,0.000025364849,0.0000036010877,5.57486e-7,4.476707e-7,0.00006764488,0.0000042198776,0.0002290799],"genre_scores_gemma":[0.99970835,0.00001136635,0.00002875537,0.000003574187,9.355792e-7,3.7107776e-7,0.00016110954,0.000002092857,0.00008336409],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998863,0.000012499631,0.0000057605075,0.000041387702,0.000026692058,0.000027463035],"domain_scores_gemma":[0.99947757,0.00007398238,0.00020752496,0.000044543856,0.00007171624,0.0001245996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015146032,0.00013488057,0.00016562387,0.0008124131,0.00020130683,0.0004955074,0.00026003193,0.00020473829,0.0013317632],"category_scores_gemma":[0.0005103153,0.00009485129,0.00013378079,0.0004098227,0.00023520578,0.00021380946,0.0005088751,0.00014420375,0.00023121241],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005514885,0.00007654619,0.94270056,0.00003290101,0.00007148913,0.00029101476,0.0005632251,0.0004466273,0.047646277,0.000096015465,0.00014308444,0.0073807454],"study_design_scores_gemma":[0.0000018472361,0.00002865587,0.9986386,0.0000018030431,0.0000074961686,0.000046750276,0.000096807504,0.0001436215,0.00091515627,0.000010225831,0.00010777577,0.0000012815178],"about_ca_topic_score_codex":0.0060693417,"about_ca_topic_score_gemma":0.0071062925,"teacher_disagreement_score":0.0060693417,"about_ca_system_score_codex":0.00022661818,"about_ca_system_score_gemma":0.00005716529,"threshold_uncertainty_score":0.012068033},"labels":[],"label_agreement":null},{"id":"W3039466905","doi":"10.3847/1538-4357/abbc1c","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Estimating Masses of Black Holes in Quasars with Single-epoch Spectroscopy","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; Natural Sciences and Engineering Research Council of Canada; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Max-Planck-Institut für Astrophysik; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Reverberation mapping; Active galactic nucleus; Quasar; Luminosity; Black hole (networking); Sky; Line (geometry); Doppler effect; Emission spectrum","score_opus":0.020532333964212345,"score_gpt":0.23444500227115464,"score_spread":0.2139126683069423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3039466905","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98954135,0.00015458382,0.0034326827,0.000056031684,0.000007589995,0.000045157918,0.0059501403,0.00020713377,0.00060536497],"genre_scores_gemma":[0.9757766,0.00010883434,0.010575733,0.000023308674,0.000015586758,0.000058532263,0.012894396,0.000031967378,0.00051503704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995449,0.00015723516,0.000027766891,0.00009740819,0.00011309908,0.0000595102],"domain_scores_gemma":[0.99820733,0.00023051072,0.00057608535,0.00038331992,0.00033098966,0.00027172122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022442194,0.00060865923,0.00030035223,0.0027240058,0.0002513473,0.00058083475,0.0006212155,0.00036471104,0.0006329019],"category_scores_gemma":[0.0024495963,0.00020752147,0.00031637144,0.0010331258,0.00020305277,0.00050838786,0.0009911342,0.00018794843,0.00040060823],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016774074,0.00008812171,0.95628965,0.000046244546,0.00022082079,0.000118713564,0.00015700213,0.004792829,0.002118011,0.00012815888,0.0019982199,0.033874575],"study_design_scores_gemma":[0.00001841802,0.0000567853,0.9797569,0.000012676993,0.000035321464,0.000098717646,0.00016137351,0.016784737,0.001643348,0.00012595065,0.0012942512,0.000011596763],"about_ca_topic_score_codex":0.018145207,"about_ca_topic_score_gemma":0.022937268,"teacher_disagreement_score":0.018145207,"about_ca_system_score_codex":0.0002724807,"about_ca_system_score_gemma":0.00030258024,"threshold_uncertainty_score":0.03607917},"labels":[],"label_agreement":null},{"id":"W3040196433","doi":"10.3847/1538-4357/aba270","title":"White Dwarfs in the Era of the LSST and Its Synergies with Space-based Missions","year":2020,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Large Synoptic Survey Telescope; Physics; Parallax; Observatory; Stars; Astronomy; James Webb Space Telescope; Galaxy; Luminosity; Astrometry; Spitzer Space Telescope; Luminosity function; Virtual observatory; Field (mathematics); Astrophysics","score_opus":0.01440555212995863,"score_gpt":0.22508619189083662,"score_spread":0.21068063976087797,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3040196433","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.983205,0.00079170056,0.00849233,0.0009896011,0.00002636192,0.000010549871,0.00021690504,0.00008051714,0.0061870157],"genre_scores_gemma":[0.9975183,0.00017390621,0.0016643063,0.000054793036,0.000013270834,0.0000031639263,0.000108688015,0.000015293423,0.00044828592],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99962044,0.0001642937,0.000013505443,0.00007660072,0.000071906616,0.000053373715],"domain_scores_gemma":[0.9987709,0.00038190937,0.0002613324,0.00022395598,0.00014691945,0.00021496617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015516771,0.0001889882,0.00029421566,0.00042106523,0.00035512177,0.0012666453,0.0003712702,0.00041658204,0.0011122497],"category_scores_gemma":[0.0029470928,0.0001481913,0.00042562684,0.00060136174,0.0006480477,0.0015921898,0.0013716867,0.00031032015,0.00016136044],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022558922,0.00010456404,0.7969294,0.00007833934,0.00016658466,0.00036070152,0.0005848628,0.12418794,0.003482157,0.034275576,0.0017939052,0.03781041],"study_design_scores_gemma":[0.00003842232,0.00026598718,0.41565654,0.0000742296,0.000087051434,0.00052092,0.0010774671,0.53306234,0.0015487312,0.02921659,0.01839714,0.000054632834],"about_ca_topic_score_codex":0.008607032,"about_ca_topic_score_gemma":0.00837125,"teacher_disagreement_score":0.008607032,"about_ca_system_score_codex":0.0006119658,"about_ca_system_score_gemma":0.0006136698,"threshold_uncertainty_score":0.017113864},"labels":[],"label_agreement":null},{"id":"W3040830538","doi":"10.3847/1538-4357/aba431","title":"Extensive Study of a Coronal Mass Ejection with UV and White-light Coronagraphs: The Need for Multiwavelength Observations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"White light; Coronal mass ejection; Materials science; Physics; Optics; Astrophysics; Optoelectronics; Solar wind; Nuclear physics; Plasma","score_opus":0.01797487161915563,"score_gpt":0.22496382999041892,"score_spread":0.2069889583712633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3040830538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99191123,0.00055170635,0.00613666,0.000038596463,0.000009992459,0.00003836292,0.0004032963,0.000090059344,0.0008200728],"genre_scores_gemma":[0.9864753,0.0002624701,0.011908345,0.000026894759,0.00005170404,0.000022616987,0.0010168427,0.000030023592,0.00020582801],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997031,0.000057686906,0.00002371054,0.000098520315,0.00007997478,0.000036966016],"domain_scores_gemma":[0.99922776,0.00021286077,0.00013290768,0.00012875542,0.00016605097,0.00013166101],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007856659,0.00020093979,0.00022810181,0.0013157066,0.00026230607,0.00033082574,0.00023753922,0.00024793964,0.0004985587],"category_scores_gemma":[0.0005826523,0.00013579814,0.00022873598,0.0009713642,0.00012102112,0.0005889671,0.00044913683,0.00015062111,0.0001037855],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026581917,0.0003750216,0.71500623,0.00023672859,0.00020082197,0.00085754145,0.00038715376,0.0028372412,0.16969112,0.00021242042,0.0006099229,0.109319955],"study_design_scores_gemma":[0.000010492315,0.00013229754,0.9830771,0.000015139959,0.00006149791,0.00041222575,0.00019162837,0.004072528,0.009707512,0.00011050564,0.0021961723,0.000012842317],"about_ca_topic_score_codex":0.0007536842,"about_ca_topic_score_gemma":0.0019328062,"teacher_disagreement_score":0.0013157066,"about_ca_system_score_codex":0.00011185172,"about_ca_system_score_gemma":0.000117244344,"threshold_uncertainty_score":0.00415504},"labels":[],"label_agreement":null},{"id":"W3041045714","doi":"10.3847/1538-4357/ab9a40","title":"WISEA J041451.67–585456.7 and WISEA J181006.18–101000.5: The First Extreme T-type Subdwarfs?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"","keywords":"Brown dwarf; Proper motion; Motion (physics); Stellar classification; Population; Planet","score_opus":0.028287828667286054,"score_gpt":0.22312460116013252,"score_spread":0.19483677249284648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041045714","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9917419,0.00024948388,0.00053611567,0.00021018149,0.00006070547,0.000009536445,0.00063428894,0.00012316533,0.006434569],"genre_scores_gemma":[0.9968328,0.00008544472,0.0006491455,0.00012301352,0.000039599036,0.0000067321853,0.0011475815,0.000029348274,0.0010863524],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991703,0.0000040650707,0.0000048270044,0.000030540647,0.000018709601,0.000024821724],"domain_scores_gemma":[0.9996112,0.000023942619,0.000116687734,0.00005691507,0.000045673267,0.00014572646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018568816,0.00023634417,0.00023893914,0.0006341995,0.0007121728,0.0007699461,0.0003191482,0.0004104827,0.0028210888],"category_scores_gemma":[0.0004327672,0.00016081992,0.00022993381,0.0004556941,0.00046141274,0.0003994948,0.00066411274,0.00044626815,0.0013589303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006012143,0.0000932813,0.8943817,0.000092541784,0.00009149121,0.0021077606,0.0011962374,0.0003950244,0.06316396,0.002039217,0.006343621,0.029493943],"study_design_scores_gemma":[0.00003419115,0.000083200466,0.97425336,0.000020771176,0.000038777216,0.0013082633,0.00080073834,0.0006343212,0.0045010787,0.0006845983,0.017622713,0.000017854834],"about_ca_topic_score_codex":0.002629501,"about_ca_topic_score_gemma":0.003982705,"teacher_disagreement_score":0.0028210888,"about_ca_system_score_codex":0.000285784,"about_ca_system_score_gemma":0.00013634242,"threshold_uncertainty_score":0.009437501},"labels":[],"label_agreement":null},{"id":"W3041250227","doi":"10.3847/1538-4357/ab9102","title":"Sensitivity of the Atmospheric Water Cycle within the Habitable Zone of a Tidally Locked, Earth-like Exoplanet","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Circumstellar habitable zone; Exoplanet; Planet; Tidal locking; Water cycle; Precipitation; Atmospheric circulation; Irradiance","score_opus":0.006838538781871442,"score_gpt":0.18294693530021763,"score_spread":0.1761083965183462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041250227","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988734,0.000013130773,0.00042228634,0.000041909898,0.000005271104,0.0000041844337,0.000070558475,0.000021220256,0.0005480399],"genre_scores_gemma":[0.9997757,0.0000074038726,0.00009642772,0.000010002042,9.949796e-7,0.0000023826724,0.00004151919,0.0000042700694,0.000061433406],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999393,0.000014603346,0.0000039051056,0.000018704202,0.0000075124713,0.000015967791],"domain_scores_gemma":[0.99976,0.0000976226,0.000036792295,0.000032240998,0.000020888541,0.00005243862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016263714,0.00021109087,0.00026834797,0.00017284758,0.00028900267,0.0005285678,0.00045140035,0.0004403365,0.0011152442],"category_scores_gemma":[0.0008641956,0.00014723718,0.00037914322,0.00011786243,0.00045096807,0.00035110407,0.0005184208,0.00041081387,0.00005229135],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042874744,0.00021142254,0.04381735,0.000040123265,0.00020039776,0.00022298069,0.00008789975,0.9160873,0.03537698,0.00105574,0.0002955784,0.0021754475],"study_design_scores_gemma":[0.00012680229,0.00028868037,0.025584087,0.0000068561676,0.000054570803,0.000041132374,0.00010409494,0.9672368,0.005618121,0.0005988203,0.00031521215,0.000024690384],"about_ca_topic_score_codex":0.011616377,"about_ca_topic_score_gemma":0.004568477,"teacher_disagreement_score":0.011616377,"about_ca_system_score_codex":0.00038439414,"about_ca_system_score_gemma":0.0002956993,"threshold_uncertainty_score":0.023097515},"labels":[],"label_agreement":null},{"id":"W3041373740","doi":"10.3847/1538-4357/aba51d","title":"The MAVERIC Survey: Chandra/ACIS Catalog of Faint X-Ray Sources in 38 Galactic Globular Clusters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Australian Government; National Aeronautics and Space Administration; National Science Foundation","keywords":"Globular cluster; Millisecond pulsar; Neutron star; Active galactic nucleus; Photometry (optics); Pulsar; Stars","score_opus":0.018050823820494492,"score_gpt":0.22553293242287972,"score_spread":0.20748210860238522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041373740","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928478,0.0005350087,0.00008069654,0.00003524806,0.000002765442,0.000022258591,0.004971636,0.000049626735,0.0014551256],"genre_scores_gemma":[0.98302025,0.0007935403,0.0008129286,0.00005266903,0.000018859499,0.000026948906,0.0144821005,0.000019047375,0.00077365804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971634,0.000020541886,0.000035260804,0.000090511174,0.00007845014,0.0000588479],"domain_scores_gemma":[0.9990283,0.00006406365,0.00030794722,0.00014399264,0.00018891193,0.0002668067],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034298384,0.0003182385,0.0002279418,0.0045350916,0.00051542214,0.0007597183,0.000496267,0.00018823377,0.0012728658],"category_scores_gemma":[0.0008311531,0.00016833753,0.00015643054,0.004098816,0.00018533404,0.00036282488,0.0009512623,0.00013647886,0.00038528725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041976346,0.000026437465,0.98289156,0.00003125736,0.000047723555,0.00014628928,0.0003616833,0.00020042456,0.0029921227,0.0001490263,0.0022350545,0.010876484],"study_design_scores_gemma":[0.0000043567425,0.000011624342,0.99696857,0.000011468269,0.000011472534,0.00015190936,0.000128219,0.00010933329,0.0002001064,0.000015625368,0.0023845176,0.0000027483136],"about_ca_topic_score_codex":0.02544456,"about_ca_topic_score_gemma":0.047794376,"teacher_disagreement_score":0.02544456,"about_ca_system_score_codex":0.00042115917,"about_ca_system_score_gemma":0.0004718587,"threshold_uncertainty_score":0.0505929},"labels":[],"label_agreement":null},{"id":"W3041833593","doi":"10.3847/1538-4357/abd6f0","title":"Maps of Magnetic Field Strength in the OMC-1 Using HAWC+ FIR Polarimetric Data","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Magnetic field; Zeeman effect; Polarimetry; Polarization (electrochemistry); Faraday effect; Molecular cloud; Field strength; Stokes parameters","score_opus":0.02991865517687265,"score_gpt":0.2762787605979434,"score_spread":0.24636010542107073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041833593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99453694,0.000055682623,0.00035554575,0.000021955097,0.0000048456695,0.000016492104,0.002207098,0.00006684636,0.002734581],"genre_scores_gemma":[0.99546224,0.000029464833,0.001239077,0.000010679335,0.000007304982,0.000008407477,0.002913695,0.000017115795,0.00031196917],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988735,0.000006609906,0.0000039223023,0.00003575463,0.000032114982,0.00003422707],"domain_scores_gemma":[0.9996171,0.00003520811,0.0000973647,0.000044689266,0.00011648928,0.000089084475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018525701,0.0002557727,0.00021936193,0.0017403805,0.00030463506,0.00047346717,0.00024109022,0.00020085301,0.0014238104],"category_scores_gemma":[0.00034419677,0.00011773236,0.00013662809,0.0010984113,0.00017658123,0.00013793344,0.0004008414,0.0002194929,0.0003159073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047617318,0.000094138224,0.8008083,0.00009221255,0.00011055094,0.0005510205,0.0005072851,0.004104447,0.1452247,0.00043205777,0.0023423207,0.045256875],"study_design_scores_gemma":[0.0000074380064,0.000011187749,0.9947608,0.000006398237,0.000006397077,0.000039748,0.00006740342,0.0019113871,0.0023738919,0.000036053894,0.0007749162,0.000004462746],"about_ca_topic_score_codex":0.018900972,"about_ca_topic_score_gemma":0.028285678,"teacher_disagreement_score":0.018900972,"about_ca_system_score_codex":0.00049438875,"about_ca_system_score_gemma":0.00023199058,"threshold_uncertainty_score":0.03758186},"labels":[],"label_agreement":null},{"id":"W3041989541","doi":"10.3847/1538-4357/ab91a4","title":"THEMIS: A Parameter Estimation Framework for the Event Horizon Telescope","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; Institut Périmètre de physique théorique; Recruitment Program of Global Experts; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; China Scholarship Council; National Research Foundation of Korea; Generalitat Valenciana; Instituto de Astrofísica de Andalucía; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Consejo Nacional de Ciencia y Tecnología; Chinese Academy of Sciences; Office of International Science and Engineering; Max-Planck-Gesellschaft; Ministerio de Economía y Competitividad; Vetenskapsrådet; John Templeton Foundation; National Radio Astronomy Observatory; U.S. Department of Energy; National Natural Science Foundation of China; Toray Science Foundation; National Research Foundation; Academia Sinica; European Commission; National Institutes of Natural Sciences; Nuclear Safety and Security Commission; Istituto Nazionale di Fisica Nucleare; Department of Science and Technology, Ministry of Science and Technology, India; Ministerio de Ciencia, Innovación y Universidades; Gordon and Betty Moore Foundation; Russian Science Foundation; Leverhulme Trust; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Government of Canada; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Supermassive black hole; Variety (cybernetics); Event (particle physics); Black hole (networking); Telescope; Set (abstract data type); Astrophysics; Computer science; Galaxy; Artificial intelligence","score_opus":0.023367944971800433,"score_gpt":0.2679665358167328,"score_spread":0.24459859084493235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3041989541","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0010591974,0.00013183702,0.9966162,0.00012530657,0.000019892555,0.000033172997,0.0002779078,0.0010752643,0.000661321],"genre_scores_gemma":[0.103396125,0.00046151585,0.8906271,0.00014851491,0.00024218432,0.00043393564,0.0020340122,0.000979935,0.0016766541],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99725753,0.0012238928,0.0001566445,0.00034545522,0.00085707207,0.00015941172],"domain_scores_gemma":[0.9956957,0.0024430605,0.0003976063,0.0005202082,0.00073373853,0.00020955007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007673666,0.0016965896,0.0015818961,0.0021791344,0.001106943,0.003682368,0.0048096315,0.0014479368,0.006454772],"category_scores_gemma":[0.016032148,0.0014333916,0.0022688846,0.0015949468,0.0013947476,0.0024302145,0.00460001,0.003382748,0.002140796],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001338259,0.00006926395,0.003264302,0.00017074822,0.0001864325,0.00021270134,0.00017379128,0.6556692,0.0013653105,0.2662274,0.0065009217,0.06602619],"study_design_scores_gemma":[0.000010291283,0.000010668348,0.00010899973,0.000014376931,0.0000062194345,0.000018933892,0.000015297976,0.95732903,0.00021607321,0.03988469,0.0023759862,0.000009379868],"about_ca_topic_score_codex":0.017115341,"about_ca_topic_score_gemma":0.01255483,"teacher_disagreement_score":0.017115341,"about_ca_system_score_codex":0.0020311447,"about_ca_system_score_gemma":0.0028753963,"threshold_uncertainty_score":0.040582716},"labels":[],"label_agreement":null},{"id":"W3042133664","doi":"10.3847/1538-4357/abb80d","title":"Constraints on Circumgalactic Media from Sunyaev–Zel’dovich Effects and X-Ray Data","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Key Research and Development Program of China; National Natural Science Foundation of China; National Science Foundation","keywords":"Halo; Virial theorem; Physics; Sunyaev–Zel'dovich effect; Astrophysics; Baryon; Galaxy; Galaxy cluster; Dark matter; Kinetic energy; Component (thermodynamics); Thermodynamics","score_opus":0.015996063491850444,"score_gpt":0.22303679749688832,"score_spread":0.20704073400503786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3042133664","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967709,0.00021473404,0.0008628393,0.00002645813,0.0000029575563,0.0000035933656,0.00028421145,0.000012248925,0.001822062],"genre_scores_gemma":[0.99957603,0.000050225604,0.00013113164,0.0000061101764,0.0000038526405,0.0000016141561,0.00019419703,0.000002635001,0.000034333134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962187,0.000106889536,0.000027596003,0.000065766064,0.00009343516,0.00008440633],"domain_scores_gemma":[0.9964091,0.0017423605,0.0007890385,0.0004858108,0.00015222747,0.00042132408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011354586,0.00042923793,0.00046024908,0.0011595467,0.0003688067,0.0013014551,0.0004116634,0.00023383889,0.0015612064],"category_scores_gemma":[0.0033039136,0.0003123894,0.00038504472,0.00050115376,0.00065768935,0.0006525416,0.00097507023,0.00021909772,0.00016198757],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004714499,0.00003765987,0.9544077,0.00009982474,0.00023846005,0.0002186159,0.00033788828,0.011970319,0.021046776,0.0044930815,0.00019732265,0.00648091],"study_design_scores_gemma":[0.000037131933,0.000046141155,0.9768196,0.000038481114,0.000079227015,0.00006768811,0.00015378639,0.013526106,0.0063753994,0.0019774323,0.00085596606,0.000022983819],"about_ca_topic_score_codex":0.00396483,"about_ca_topic_score_gemma":0.0048639057,"teacher_disagreement_score":0.00396483,"about_ca_system_score_codex":0.0005479635,"about_ca_system_score_gemma":0.00019437655,"threshold_uncertainty_score":0.007883549},"labels":[],"label_agreement":null},{"id":"W3042212797","doi":"10.3847/1538-4357/abb1b1","title":"Probing the Growth of Massive Black Holes with Black Hole–Host Galaxy Spin Correlations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Galaxy; Black hole (networking); Spins; Redshift; Galaxy formation and evolution; Spin-flip; Supermassive black hole; Spin (aerodynamics)","score_opus":0.009408216902549133,"score_gpt":0.2048764407611526,"score_spread":0.19546822385860346,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3042212797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99886715,0.000053187006,0.0005030106,0.000014005461,0.0000016405656,0.000002247577,0.00007220675,0.000013915739,0.00047258136],"genre_scores_gemma":[0.99963117,0.000010559118,0.00025955788,0.00000480512,0.0000021699577,8.404605e-7,0.000041367948,0.0000017599519,0.000047819038],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989915,0.000019399977,0.0000026714188,0.000027816337,0.000014503096,0.000036458554],"domain_scores_gemma":[0.9993223,0.00012404357,0.00030177087,0.000060287268,0.00005991374,0.00013171893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034672863,0.00017738671,0.00011813033,0.0007536749,0.00015899148,0.00038301913,0.00018685362,0.00020021724,0.0008448235],"category_scores_gemma":[0.00077657157,0.00013049414,0.0001203167,0.00031266588,0.0002879858,0.00034088775,0.00038097636,0.0002005872,0.00012024823],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021582656,0.000059804057,0.89302796,0.000027029888,0.000073538926,0.00019310733,0.00016608676,0.0010259678,0.09639671,0.0012913422,0.00022894041,0.0072937007],"study_design_scores_gemma":[0.000008948002,0.00009283272,0.9722387,0.000006153703,0.000029846393,0.00023537454,0.00015888903,0.009640389,0.016537908,0.00064058055,0.00039784505,0.000012439692],"about_ca_topic_score_codex":0.00069863506,"about_ca_topic_score_gemma":0.0010718671,"teacher_disagreement_score":0.0008448235,"about_ca_system_score_codex":0.00016708237,"about_ca_system_score_gemma":0.00006529219,"threshold_uncertainty_score":0.0028262734},"labels":[],"label_agreement":null},{"id":"W3042241317","doi":"10.3847/1538-4357/abb377","title":"The Cepheid Distance to the Seyfert 1 Galaxy NGC 4151","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Cepheid variable; Galaxy; Supermassive black hole; Hubble space telescope; Hubble sequence; Hubble's law; Active galactic nucleus","score_opus":0.008257151150042233,"score_gpt":0.20679396932401647,"score_spread":0.19853681817397423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3042241317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99336433,0.00031498435,0.00021236924,0.00009312572,0.00001048291,0.0000016496972,0.00036050676,0.000013973713,0.005628486],"genre_scores_gemma":[0.9985771,0.00009240594,0.0001274712,0.000013160308,0.000006102929,0.0000014728665,0.00035570262,0.0000023128125,0.00082420517],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991846,0.000006690409,0.000003328296,0.000029002507,0.000022607239,0.000019902245],"domain_scores_gemma":[0.9997002,0.00004718503,0.00008141063,0.000029147024,0.00005214441,0.00008987382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010323277,0.00012573901,0.000108227956,0.0008228049,0.0005796656,0.0005005355,0.00024678212,0.0002665732,0.0043924884],"category_scores_gemma":[0.0005843098,0.00007030621,0.000068572845,0.00037322732,0.00025421722,0.00032570804,0.00042853082,0.00029763082,0.0007623255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001655064,0.000035492103,0.93591523,0.00008755334,0.0000586368,0.00056081126,0.00093626906,0.002232031,0.018422637,0.005306071,0.0023460898,0.033933695],"study_design_scores_gemma":[0.000002950224,0.000016370534,0.9951108,0.00000957596,0.0000064511673,0.00021607861,0.00017464004,0.0004535612,0.00060664926,0.00046453017,0.0029336258,0.000004765583],"about_ca_topic_score_codex":0.011129677,"about_ca_topic_score_gemma":0.013184297,"teacher_disagreement_score":0.011129677,"about_ca_system_score_codex":0.00052345253,"about_ca_system_score_gemma":0.00016674178,"threshold_uncertainty_score":0.022129774},"labels":[],"label_agreement":null},{"id":"W3042512578","doi":"10.3847/1538-4357/abb085","title":"The Completed SDSS-IV Extended Baryon Oscillation Spectroscopic Survey: Baryon Acoustic Oscillations with Lyα Forests","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":358,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Agence Nationale de la Recherche; University of Oxford; York University; National Energy Research Scientific Computing Center; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ministerio de Ciencia e Innovación; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Quasar; Baryon acoustic oscillations; Baryon; Redshift; Oscillation (cell signaling); Cosmology; Measure (data warehouse); Autocorrelation","score_opus":0.01426917288340995,"score_gpt":0.22643204100910844,"score_spread":0.21216286812569848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3042512578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8596547,0.00029208342,0.003815791,0.00020429523,0.00004229292,0.0000963959,0.12522745,0.00052049145,0.010146488],"genre_scores_gemma":[0.7781134,0.00019595076,0.00828541,0.00019664865,0.00012691773,0.00012877559,0.20786726,0.00018536275,0.0049003204],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995029,0.00010293448,0.000031686355,0.00010876828,0.00017479013,0.00007886895],"domain_scores_gemma":[0.9982718,0.00014669655,0.0004333293,0.00037791545,0.0003727429,0.00039752474],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010795827,0.00031812265,0.00030664977,0.0016480373,0.00020934407,0.00062808173,0.00032910623,0.00015912858,0.0024753697],"category_scores_gemma":[0.0015259847,0.00017867342,0.00023681243,0.0015471617,0.00016794057,0.00025890954,0.0009782736,0.0003056571,0.0015068171],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029936226,0.00012745838,0.92119867,0.00010384036,0.00019127,0.00007117194,0.0002976457,0.0020074109,0.011829015,0.0013679629,0.029869668,0.03263659],"study_design_scores_gemma":[0.000026524205,0.000028822686,0.98036456,0.000014882321,0.000024945955,0.00003777717,0.00006249208,0.0010725685,0.0010820446,0.00027455276,0.016999198,0.000011551443],"about_ca_topic_score_codex":0.01647848,"about_ca_topic_score_gemma":0.019294498,"teacher_disagreement_score":0.01647848,"about_ca_system_score_codex":0.00039061785,"about_ca_system_score_gemma":0.00048730776,"threshold_uncertainty_score":0.03276515},"labels":[],"label_agreement":null},{"id":"W3043088937","doi":"10.3847/1538-4357/aba437","title":"On the Possibility of Detecting Helium D3 Line Polarization with Metis","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council","keywords":"Physics; Thomson scattering; Polarization (electrochemistry); Linear polarization; Metis; Solar prominence; Scattering; Helium; Magnetic field; Atomic physics; Circular polarization; Orbiter; Astrophysics; Optics; Astronomy; Chemistry; Laser","score_opus":0.009934273997020187,"score_gpt":0.21516644167749005,"score_spread":0.20523216768046987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3043088937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9901175,0.000063235355,0.0073214974,0.00008146984,0.0000065553663,0.0000067529822,0.00023559156,0.0003331241,0.0018342081],"genre_scores_gemma":[0.99719775,0.000010912907,0.0024925803,0.000006709021,0.000001314834,0.0000022414124,0.00011423074,0.00001545224,0.00015877603],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999355,0.0000127797175,0.0000016468405,0.000012918539,0.000021265601,0.000015934142],"domain_scores_gemma":[0.9997787,0.00012798964,0.000022762166,0.00001882944,0.000030617895,0.000021145004],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018472607,0.00023830871,0.00018427976,0.00022858077,0.000201763,0.00037449133,0.00039333967,0.00031446764,0.0014725863],"category_scores_gemma":[0.000495548,0.00015222261,0.0002835082,0.00025589173,0.00022686941,0.0002961225,0.00024204745,0.0002736387,0.00010498524],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012069799,0.0001583527,0.15386227,0.00012052343,0.00010663873,0.00050115073,0.00014789643,0.72991246,0.08707303,0.0029959315,0.0011608652,0.022753859],"study_design_scores_gemma":[0.000029882409,0.0000816493,0.017256524,0.0000050349686,0.000012328482,0.000039686114,0.000031512907,0.96228427,0.01941563,0.00051151594,0.00032232524,0.00000965175],"about_ca_topic_score_codex":0.0043904437,"about_ca_topic_score_gemma":0.0037612177,"teacher_disagreement_score":0.0043904437,"about_ca_system_score_codex":0.00040731483,"about_ca_system_score_gemma":0.00017633609,"threshold_uncertainty_score":0.0087298155},"labels":[],"label_agreement":null},{"id":"W3043705672","doi":"10.3847/1538-4357/ab9c1f","title":"Hybrid Very Long Baseline Interferometry Imaging and Modeling with themis","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Government of Canada; Ministère de l'Économie, de la Science et de l'Innovation - Québec; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada; Natural Sciences and Engineering Research Council of Canada; Université de Sherbrooke; Compute Canada; Harvard University; Ministero dello Sviluppo Economico; Gordon and Betty Moore Foundation; John Templeton Foundation","keywords":"Physics; Bayesian probability; Interferometry; Inverse problem; Artificial intelligence; Iterative reconstruction; Smoothness; Computer vision; Algorithm; Optics; Computer science","score_opus":0.01472345759981142,"score_gpt":0.28461458073412466,"score_spread":0.26989112313431324,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3043705672","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.071435735,0.000111136025,0.92538154,0.0001957527,0.000015942296,0.000019827059,0.00022608161,0.00053518236,0.0020787937],"genre_scores_gemma":[0.83395207,0.00011458388,0.16363166,0.000060678638,0.000030584666,0.000055964436,0.0004236941,0.00013715308,0.0015936437],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998024,0.000060416693,0.0000098556075,0.00003716968,0.0000676331,0.000022531416],"domain_scores_gemma":[0.9995827,0.00019675467,0.0000877789,0.00006716526,0.00004637854,0.000019185505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006195694,0.0003450173,0.00036490004,0.00040242748,0.00021515139,0.00077482266,0.0009557647,0.00064120186,0.0009140317],"category_scores_gemma":[0.0012738094,0.000435286,0.00057030784,0.00045304513,0.00050863915,0.0008437833,0.0006001124,0.0006754713,0.00019600987],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000028487886,0.000019585133,0.0014309674,0.000017207687,0.0000346353,0.00003149814,0.000027292068,0.9728602,0.0040947944,0.011073609,0.00021634168,0.010165287],"study_design_scores_gemma":[0.0000016983092,0.000004486199,0.0002743303,0.0000014206845,0.0000016455682,0.000007797864,0.0000022089228,0.9975169,0.000508307,0.0014814622,0.00019629076,0.000003495132],"about_ca_topic_score_codex":0.0055498956,"about_ca_topic_score_gemma":0.0046978816,"teacher_disagreement_score":0.0055498956,"about_ca_system_score_codex":0.0006324171,"about_ca_system_score_gemma":0.00054807763,"threshold_uncertainty_score":0.011035204},"labels":[],"label_agreement":null},{"id":"W3044868348","doi":"10.3847/1538-4357/ab96c6","title":"Verification of Radiative Transfer Schemes for the EHT","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; University of Waterloo; Perimeter Institute","funders":"Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Recruitment Program of Global Experts; China Scholarship Council; Office of International Science and Engineering; Max-Planck-Gesellschaft; National Research Foundation of Korea; National Radio Astronomy Observatory; John Templeton Foundation; National Natural Science Foundation of China; Vetenskapsrådet; Generalitat Valenciana; Chinese Academy of Sciences; Harvard University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministry of Education, Culture, Sports, Science and Technology; National Research Foundation; European Commission; National Institutes of Natural Sciences; Nuclear Safety and Security Commission; Istituto Nazionale di Fisica Nucleare; Department of Science and Technology, Ministry of Science and Technology, India; Gordon and Betty Moore Foundation; Leverhulme Trust; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Consejo Nacional de Ciencia y Tecnología; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Government of Canada; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Radiative transfer; Astrophysics; Astronomy; Optics","score_opus":0.027288651177919395,"score_gpt":0.24486003177177565,"score_spread":0.21757138059385625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3044868348","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.82154703,0.00011782422,0.16617809,0.00029540015,0.00009710886,0.00013652086,0.00053142017,0.0030833287,0.008013357],"genre_scores_gemma":[0.9657497,0.000019977624,0.033294838,0.00003286383,0.0000104437,0.000042142336,0.00019294138,0.00020442888,0.0004525727],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99842536,0.0005819873,0.00012415997,0.00019939664,0.00050835375,0.00016084356],"domain_scores_gemma":[0.99045205,0.004175931,0.00064858765,0.002813266,0.0016606859,0.00024953278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0034755229,0.00047237374,0.00042694123,0.00043738988,0.0006681828,0.0008607448,0.0016987976,0.00087956054,0.0014607371],"category_scores_gemma":[0.018069534,0.00020662708,0.0005605085,0.0004021169,0.0012208173,0.0011983395,0.0013904732,0.00083721004,0.00024054905],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000525128,0.00021338086,0.018679684,0.000097647426,0.00007996008,0.00021050166,0.00033740915,0.901489,0.010349978,0.04506547,0.0009233767,0.022028439],"study_design_scores_gemma":[0.000044792796,0.000053064676,0.00084579777,0.000005227854,0.000005535644,0.000021707923,0.000025018118,0.9897597,0.00525152,0.0035716633,0.00040789967,0.000008068015],"about_ca_topic_score_codex":0.006926308,"about_ca_topic_score_gemma":0.0018349199,"teacher_disagreement_score":0.006926308,"about_ca_system_score_codex":0.0013102244,"about_ca_system_score_gemma":0.0011273399,"threshold_uncertainty_score":0.018380523},"labels":[],"label_agreement":null},{"id":"W3044963766","doi":"10.3847/1538-4357/aba433","title":"The Next Generation Virgo Cluster Survey (NGVS). XXX. Ultra-diffuse Galaxies and Their Globular Cluster Systems","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":109,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea; National Natural Science Foundation of China","keywords":"Virgo Cluster; Globular cluster; Galaxy; Galaxy cluster; Coma Cluster; Cluster (spacecraft); Dwarf galaxy","score_opus":0.023373302586543847,"score_gpt":0.21236063685938902,"score_spread":0.18898733427284517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3044963766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9857491,0.0011283355,0.00040739836,0.000068874004,0.0000067084125,0.000026490721,0.007751391,0.000034216147,0.00482749],"genre_scores_gemma":[0.9844557,0.00031328897,0.0006620077,0.000040692878,0.000009554997,0.00001829919,0.013149046,0.000010333414,0.001341182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998129,0.000030015326,0.000009069459,0.00004739068,0.000048143083,0.00005247642],"domain_scores_gemma":[0.9997018,0.000031811636,0.000088292116,0.000044460427,0.000040040897,0.00009360506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023717193,0.00015994426,0.00016328196,0.0022331679,0.00028384276,0.00050101284,0.0002550215,0.00014625392,0.0014390834],"category_scores_gemma":[0.00053277845,0.00008242262,0.00017066745,0.0023396604,0.00021313797,0.00028371534,0.0006447441,0.00015136908,0.00046406905],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041050513,0.000014008353,0.98594046,0.00002096579,0.00002555027,0.00003976734,0.00015016885,0.00019078623,0.0011929446,0.00043800744,0.0012077044,0.010738617],"study_design_scores_gemma":[7.5968927e-7,0.00000455136,0.997938,0.0000028529334,0.0000032917203,0.000031563668,0.000057637906,0.00014231683,0.000069798894,0.000056962923,0.0016910434,0.0000010896305],"about_ca_topic_score_codex":0.02807711,"about_ca_topic_score_gemma":0.040892836,"teacher_disagreement_score":0.02807711,"about_ca_system_score_codex":0.0005678491,"about_ca_system_score_gemma":0.00020638804,"threshold_uncertainty_score":0.05582738},"labels":[],"label_agreement":null},{"id":"W3044997459","doi":"10.3847/1538-4357/ac033a","title":"HInet: Generating Neutral Hydrogen from Dark Matter with Neural Networks","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Mila - Quebec Artificial Intelligence Institute","funders":"","keywords":"Dark matter; Nonlinear system; Halo; Convolutional neural network; Artificial neural network; Distribution (mathematics); COSMIC cancer database; Cosmology; Neutral network","score_opus":0.005410984760446328,"score_gpt":0.18889431271221543,"score_spread":0.1834833279517691,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3044997459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58757347,0.0007461528,0.36991012,0.001234991,0.0004970314,0.0002624621,0.006089907,0.022829114,0.010856786],"genre_scores_gemma":[0.90601295,0.00010471154,0.08534347,0.000262053,0.00008158086,0.0001561832,0.0042954707,0.00050340546,0.003240124],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991477,0.000027402128,0.000003538327,0.000023276229,0.000016478314,0.000014542824],"domain_scores_gemma":[0.9995944,0.00023849864,0.000034106335,0.000049080252,0.00004842239,0.000035570458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040912398,0.00067706325,0.00034387354,0.00056373444,0.00032091388,0.00051500346,0.0010208188,0.00086597895,0.0033618212],"category_scores_gemma":[0.0019722541,0.00036546472,0.0005189397,0.00043686296,0.00037125696,0.0004600407,0.0007238538,0.0006302954,0.0005526419],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012807276,0.00006038402,0.0027338022,0.00006124048,0.00008099494,0.000100594705,0.000025654914,0.96775603,0.0016615968,0.0030000843,0.003984328,0.020407306],"study_design_scores_gemma":[0.000010980168,0.0000062615277,0.00016735277,0.000001642911,0.0000022199454,0.0000035502042,0.0000020048747,0.99778277,0.00050828804,0.0013164319,0.00019650062,0.000002072072],"about_ca_topic_score_codex":0.008797768,"about_ca_topic_score_gemma":0.007381891,"teacher_disagreement_score":0.008797768,"about_ca_system_score_codex":0.00071276654,"about_ca_system_score_gemma":0.00047592938,"threshold_uncertainty_score":0.017493129},"labels":[],"label_agreement":null},{"id":"W3045177582","doi":"10.3847/1538-4357/abb8dd","title":"A Strong-lensing Model for the WMDF JWST/GTO Very Rich Cluster A1489","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Agencia Nacional de Investigación y Desarrollo; Ben-Gurion University of the Negev; University of Oxford; York University; Ministerio de Ciencia, Innovación y Universidades; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Goddard Space Flight Center; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ministero dell’Istruzione, dell’Università e della Ricerca; Carnegie Mellon University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Agencia Estatal de Investigación; Yale University","keywords":"ROSAT; Einstein radius; Galaxy; Redshift; Galaxy cluster; Luminosity; Cluster (spacecraft); Mass distribution; Cosmology; RADIUS","score_opus":0.018360138223317155,"score_gpt":0.22783855795736402,"score_spread":0.20947841973404685,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3045177582","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93597066,0.00027757476,0.03866566,0.0010493299,0.000038117658,0.0000793179,0.0015269917,0.0001582566,0.022234086],"genre_scores_gemma":[0.9923316,0.000083391285,0.002830392,0.00008089802,0.000050539304,0.000046818262,0.0004714329,0.000042228174,0.0040625646],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999859,0.000032513173,0.0000049626174,0.000034349534,0.000030750434,0.00003835181],"domain_scores_gemma":[0.99968135,0.000045338395,0.00007746457,0.00003489701,0.000040511517,0.000120417586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032332394,0.00048745013,0.00041786296,0.00083611906,0.0007786954,0.0011213837,0.0013610576,0.00073995895,0.0053433776],"category_scores_gemma":[0.00077223056,0.00022496739,0.0006807467,0.00042183322,0.000625395,0.00083611696,0.00087762676,0.00043544394,0.000810336],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049030787,0.00023022945,0.098321296,0.00014132539,0.00029406775,0.0015903104,0.00064417213,0.5436964,0.019265216,0.30684865,0.014147195,0.014330789],"study_design_scores_gemma":[0.000093269875,0.000058090147,0.034315135,0.000020190926,0.000040123752,0.0002572976,0.00017041792,0.91990596,0.00052107906,0.040032484,0.004540776,0.000045111614],"about_ca_topic_score_codex":0.021516303,"about_ca_topic_score_gemma":0.012739447,"teacher_disagreement_score":0.021516303,"about_ca_system_score_codex":0.0013234579,"about_ca_system_score_gemma":0.00048178356,"threshold_uncertainty_score":0.042782128},"labels":[],"label_agreement":null},{"id":"W3045694437","doi":"10.3847/1538-4357/ac0627","title":"Revisiting Dynamical Friction: The Role of Global Modes and Local Wakes","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Dynamical friction; Astrophysics; Galaxy; Globular cluster; Dark matter; Astronomy; Dwarf galaxy; Milky Way; Orbital decay; Local Group; Dark matter halo; Halo; Drag; Galaxy formation and evolution; Satellite","score_opus":0.004203204995652643,"score_gpt":0.20249035245423153,"score_spread":0.1982871474585789,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3045694437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9769056,0.0005868832,0.012476919,0.00078356767,0.00008541548,0.000029235447,0.000095520045,0.00009021844,0.008946605],"genre_scores_gemma":[0.99874145,0.00008988881,0.00066023157,0.00003630441,0.00001732377,0.0000050561807,0.000016083242,0.000019669345,0.00041396794],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999063,0.000023468412,0.000004112517,0.000016052812,0.000016467682,0.000033523116],"domain_scores_gemma":[0.9995658,0.00017859504,0.00008261928,0.000059542894,0.000035686764,0.00007780891],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003223809,0.00041880689,0.00069515157,0.00031985214,0.0005530037,0.0012240222,0.00086779246,0.0007168941,0.0025724105],"category_scores_gemma":[0.0016192349,0.00029195845,0.0004869161,0.0002302618,0.0016724985,0.0017357938,0.001320655,0.0010671589,0.00017048074],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018575175,0.00018639182,0.02492245,0.00012991724,0.00011394218,0.0006299802,0.00046042295,0.91223246,0.009343967,0.043439403,0.001176012,0.0071793357],"study_design_scores_gemma":[0.000037582056,0.000044242806,0.0058637634,0.000014115317,0.000013434318,0.00003314799,0.00009927508,0.9879078,0.00037000285,0.005146533,0.00045626744,0.000013845206],"about_ca_topic_score_codex":0.012767244,"about_ca_topic_score_gemma":0.006787228,"teacher_disagreement_score":0.012767244,"about_ca_system_score_codex":0.0006444118,"about_ca_system_score_gemma":0.00056646735,"threshold_uncertainty_score":0.025385857},"labels":[],"label_agreement":null},{"id":"W3045792864","doi":"10.3847/1538-4357/abaab4","title":"Solving Grain Size Inconsistency between ALMA Polarization and VLA Continuum in the Ophiuchus IRS 48 Protoplanetary Disk","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Ophiuchus; Physics; Millimeter; Astrophysics; Submillimeter Array; Protoplanetary disk; Polarization (electrochemistry); Wavelength; Grain size; Molecular cloud; Stars; Star formation; Optics","score_opus":0.011858713023245879,"score_gpt":0.22458909961455895,"score_spread":0.21273038659131308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3045792864","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999265,0.000030939103,0.00019753732,0.000011139511,0.000001306768,0.0000010693649,0.000032496002,0.000009733685,0.00045070646],"genre_scores_gemma":[0.9998474,0.000005004135,0.000087163906,0.0000036377253,0.0000019379972,6.226816e-7,0.000027268039,0.000001059682,0.000025842504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992,0.000012436034,0.0000046813275,0.000027581866,0.000015867538,0.000019469851],"domain_scores_gemma":[0.99964046,0.00011078672,0.000117083306,0.00004026712,0.000051346775,0.000039914532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014637837,0.000101636135,0.00011451777,0.0005208796,0.00021254194,0.0004393265,0.0001827269,0.00020889644,0.0008099322],"category_scores_gemma":[0.00066484674,0.00012385432,0.00008090844,0.00022285046,0.00022724262,0.00025628263,0.00023527935,0.00015263045,0.00016956849],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021334343,0.000035022436,0.9096146,0.000013555484,0.000038465612,0.00023007882,0.00014711905,0.00043166545,0.08339925,0.0001975516,0.00013905883,0.005540264],"study_design_scores_gemma":[0.0000066517223,0.000022500168,0.99387014,0.0000023458306,0.000009712113,0.00015842666,0.00015501447,0.0012278861,0.0042333314,0.00016565264,0.00014613944,0.000002288587],"about_ca_topic_score_codex":0.001077438,"about_ca_topic_score_gemma":0.0012086907,"teacher_disagreement_score":0.001077438,"about_ca_system_score_codex":0.00021541392,"about_ca_system_score_gemma":0.00004948046,"threshold_uncertainty_score":0.002709508},"labels":[],"label_agreement":null},{"id":"W3046086630","doi":"10.3847/1538-4357/aba830","title":"Steady Wind-blown Cavities within Infalling Rotating Envelopes: Application to the Broad Velocity Component in Young Protostars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; European Southern Observatory; National Research Foundation; Danmarks Grundforskningsfond; Agence Nationale de la Recherche; Villum Fonden","keywords":"Protostar; Outflow; Accretion (finance); Stars; Turbulence; Envelope (radar); Entrainment (biomusicology); Thermal wind; Supermassive black hole; Jet (fluid)","score_opus":0.01452863891585491,"score_gpt":0.24222702275788785,"score_spread":0.22769838384203295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3046086630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967282,0.00004766717,0.0025350198,0.000021396656,0.0000027487831,0.0000073958267,0.000029137076,0.00007129274,0.00055714196],"genre_scores_gemma":[0.99871266,0.000015380947,0.001133324,0.0000034065054,0.0000018392814,0.0000025364345,0.00001587977,0.000008838871,0.00010614664],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999609,0.000007817879,0.0000021060328,0.000007307191,0.000008732977,0.000013099629],"domain_scores_gemma":[0.99974614,0.00009560781,0.000059945953,0.000021669077,0.000025793744,0.000050897695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020658867,0.00034264132,0.00026574437,0.00036840065,0.0004351846,0.0005157971,0.00055321294,0.0006250568,0.0008015323],"category_scores_gemma":[0.0006638264,0.00020861479,0.00037033737,0.0002624464,0.0003780006,0.00019975618,0.000412101,0.00024180365,0.000085216954],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015000031,0.0001236944,0.0768371,0.000045906767,0.000039026498,0.00095651095,0.00017828528,0.88440806,0.02918538,0.0018830993,0.00016335276,0.006029594],"study_design_scores_gemma":[0.000017749502,0.00005854016,0.016916815,0.0000046536707,0.000006058906,0.00007919448,0.00005650838,0.97996145,0.0025416904,0.00023732134,0.0001107701,0.000009262363],"about_ca_topic_score_codex":0.007817483,"about_ca_topic_score_gemma":0.0045524673,"teacher_disagreement_score":0.007817483,"about_ca_system_score_codex":0.0005552679,"about_ca_system_score_gemma":0.0003442145,"threshold_uncertainty_score":0.015543938},"labels":[],"label_agreement":null},{"id":"W3046418130","doi":"10.3847/1538-4357/ab9c1d","title":"Heuristic Description of Perpendicular Particle Transport in Turbulence with Super-diffusive Magnetic Field Lines","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Magnetic field; Statistical physics; Heuristic; Perpendicular; Diffusion; Test particle; Turbulence; Limit (mathematics); Particle (ecology); Classical mechanics; Field (mathematics); Computational physics; Mechanics; Mathematical analysis; Geometry; Mathematical optimization; Quantum mechanics","score_opus":0.00842438879073798,"score_gpt":0.19836189747728927,"score_spread":0.1899375086865513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3046418130","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.33654904,0.0009596042,0.6323308,0.0010385145,0.00030844944,0.00014875445,0.00022755416,0.00036637226,0.028070906],"genre_scores_gemma":[0.9679091,0.00025178032,0.024287555,0.00013878227,0.000081653765,0.00009091587,0.00008331262,0.000076203876,0.0070806774],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99981576,0.000049707225,0.000010612995,0.000021275613,0.0000569005,0.00004579096],"domain_scores_gemma":[0.9996381,0.00009990565,0.00008145419,0.000049763323,0.00007289539,0.000057794103],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047199882,0.0005647891,0.0006405984,0.0009819845,0.00070186367,0.0011894306,0.0012526183,0.0010713689,0.0027099547],"category_scores_gemma":[0.0010218658,0.00028704558,0.0005948469,0.00036798962,0.0010708449,0.0014870352,0.0007635109,0.0007355767,0.00030677812],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013506795,0.00010988563,0.0017235031,0.00009133988,0.000037674326,0.0008451474,0.00015405325,0.27927816,0.012361157,0.7004609,0.0011613406,0.0036417695],"study_design_scores_gemma":[0.00002026068,0.00003390981,0.00028722003,0.0000057777197,0.0000039160354,0.000084302694,0.000024411002,0.9549925,0.00038993402,0.043537755,0.0006050892,0.000014976206],"about_ca_topic_score_codex":0.0019904976,"about_ca_topic_score_gemma":0.0010697279,"teacher_disagreement_score":0.0027099547,"about_ca_system_score_codex":0.00091969344,"about_ca_system_score_gemma":0.0004827982,"threshold_uncertainty_score":0.009065688},"labels":[],"label_agreement":null},{"id":"W3046578869","doi":"10.3847/1538-4357/abac17","title":"Predicting the Kinematic Evidence of Gravitational Instability","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Australian Research Council; Science and Technology Facilities Council","keywords":"Exoplanet; Gravitational instability; Instability; Gravitation; Kinematics; Planet; Radiative transfer; Accretion (finance)","score_opus":0.029976334014999922,"score_gpt":0.2738054239356327,"score_spread":0.24382908992063276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3046578869","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99202216,0.0000765337,0.005972172,0.00008708921,0.0000053327853,0.000008993204,0.0001702021,0.00009952296,0.0015580597],"genre_scores_gemma":[0.99902797,0.000018430155,0.0008088545,0.000005376498,0.0000024788055,0.0000019490853,0.00008497321,0.0000040932796,0.00004583323],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999113,0.00002437738,0.000005637504,0.000024889398,0.000018697721,0.000015156252],"domain_scores_gemma":[0.99879646,0.0006055297,0.00032880175,0.00006881767,0.00012371018,0.000076603596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030351692,0.00026836104,0.00017893342,0.00059734733,0.00021504557,0.0008265683,0.00033409984,0.0003999826,0.0008687352],"category_scores_gemma":[0.0034113682,0.00024784816,0.00018407727,0.00030643147,0.00034542737,0.00075719226,0.0003222014,0.00023155434,0.0002459921],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012961579,0.000057109894,0.8962074,0.000022588574,0.00006426981,0.00019526358,0.00006177266,0.072735645,0.020394169,0.0023445443,0.00024012677,0.007547416],"study_design_scores_gemma":[0.000024051618,0.000062434854,0.28348777,0.000009067429,0.00002964155,0.0000955382,0.000089446934,0.7040034,0.009638408,0.0021323639,0.00041108677,0.000016804865],"about_ca_topic_score_codex":0.004604552,"about_ca_topic_score_gemma":0.002506057,"teacher_disagreement_score":0.004604552,"about_ca_system_score_codex":0.0005706093,"about_ca_system_score_gemma":0.00017580423,"threshold_uncertainty_score":0.009155512},"labels":[],"label_agreement":null},{"id":"W3046870831","doi":"10.3847/1538-4357/ababaa","title":"The Red Supergiant Binary Fraction of the Large Magellanic Cloud","year":2020,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Astrophysics; Physics; Photometry (optics); Stars; Large Magellanic Cloud; Binary number; Red supergiant; Small Magellanic Cloud; Binary star; Supergiant; Astronomy; Mathematics","score_opus":0.015398836200828183,"score_gpt":0.2734505654306708,"score_spread":0.25805172922984265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3046870831","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99784493,0.00020656291,0.0003819933,0.000019574476,0.0000021184208,0.0000020620566,0.00047917425,0.00001634361,0.0010471754],"genre_scores_gemma":[0.99939597,0.000027198836,0.00010144681,0.000004649548,0.0000025001066,7.5961674e-7,0.0003703044,0.000002219719,0.000094948475],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981123,0.000026099593,0.0000101653395,0.00005854984,0.000050239196,0.000043753218],"domain_scores_gemma":[0.99925596,0.00014081555,0.00026822998,0.00011056893,0.0001014893,0.00012294104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028178975,0.0001129178,0.00013136883,0.0012818237,0.0002881624,0.0005298051,0.00022730307,0.00012959511,0.0018206006],"category_scores_gemma":[0.0011704966,0.000077545126,0.000117033116,0.0005401578,0.0002571621,0.00036976373,0.00037373934,0.00013611652,0.00043257725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042123153,0.000006215808,0.98941725,0.000014713358,0.000029776724,0.000029464723,0.00005411485,0.00050793967,0.0031515225,0.00030195017,0.00028263472,0.006162301],"study_design_scores_gemma":[0.0000012702724,0.0000074866034,0.9969639,0.0000048847915,0.00000639477,0.000061296516,0.000055238535,0.0011931849,0.0009270298,0.00014138612,0.00063613954,0.00000162769],"about_ca_topic_score_codex":0.007926632,"about_ca_topic_score_gemma":0.009228686,"teacher_disagreement_score":0.007926632,"about_ca_system_score_codex":0.0004529313,"about_ca_system_score_gemma":0.00013313077,"threshold_uncertainty_score":0.015761018},"labels":[],"label_agreement":null},{"id":"W3046992070","doi":"10.3847/1538-4357/abd6c7","title":"Primordial Radius Gap and Potentially Broad Core Mass Distributions of Super-Earths and Sub-Neptunes","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Accretion (finance); Photoevaporation; RADIUS; Mass distribution; Exoplanet; Planet; Distribution function; Gas giant; Stars","score_opus":0.012674903347209566,"score_gpt":0.23293055552198716,"score_spread":0.2202556521747776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3046992070","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99912137,0.00010832096,0.00021622879,0.000008396638,4.5274675e-7,6.307372e-7,0.000056562058,0.000008205385,0.00047991605],"genre_scores_gemma":[0.9998024,0.000012267702,0.000061335755,0.0000024766516,7.7633996e-7,5.2996035e-7,0.00006430029,0.0000030964645,0.000052790587],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993515,0.0000069517355,0.000002918577,0.000031028874,0.000009434777,0.00001463376],"domain_scores_gemma":[0.9995832,0.00010567643,0.00012886338,0.00004937834,0.00003980164,0.0000931155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012664232,0.00008815745,0.00018066615,0.0004694855,0.00014772784,0.00039507262,0.00020695379,0.00019471043,0.00091459544],"category_scores_gemma":[0.0005955742,0.00008905052,0.00010048846,0.00016939252,0.00035175335,0.00025455194,0.00034221823,0.00019390303,0.00020588705],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008165754,0.000028555285,0.76559436,0.00004677913,0.000059042453,0.00056842424,0.00089182315,0.0015855827,0.20809472,0.0019467721,0.0002829676,0.020084484],"study_design_scores_gemma":[0.0000052053674,0.00004326389,0.9924649,0.0000029315538,0.000004322857,0.0004372554,0.00013792627,0.0015954132,0.0041559706,0.0006305678,0.00051775534,0.0000045095294],"about_ca_topic_score_codex":0.0006559438,"about_ca_topic_score_gemma":0.00052686565,"teacher_disagreement_score":0.00091459544,"about_ca_system_score_codex":0.00017101508,"about_ca_system_score_gemma":0.000039080234,"threshold_uncertainty_score":0.0030596256},"labels":[],"label_agreement":null},{"id":"W3047330737","doi":"10.3847/1538-4357/abaab8","title":"Resolving Decades of Periodic Spirals from the Wolf–Rayet Dust Factory WR 112","year":2020,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Circumstellar dust; Wolf–Rayet star; Orbital motion; Dust lane; Luminosity; Spiral galaxy; Cosmic dust; Nebula; Astronomy; Stars; Star formation; Galaxy; Angular momentum","score_opus":0.03151256649179492,"score_gpt":0.2670070663045223,"score_spread":0.23549449981272738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3047330737","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990375,0.000039962197,0.00023546586,0.000011819079,0.0000023266355,0.000002935964,0.00021100584,0.000022353783,0.0004365424],"genre_scores_gemma":[0.9989716,0.00001756418,0.00039824256,0.0000051988495,0.0000034296881,0.0000023721575,0.00047250933,0.000008072818,0.00012094404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989486,0.000008614844,0.0000065594795,0.000042584936,0.000019226247,0.000028128543],"domain_scores_gemma":[0.99962664,0.0000401418,0.00010113769,0.00005965906,0.000061168736,0.0001112765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022561547,0.00020159187,0.00021957894,0.0008245301,0.00032335322,0.0004746339,0.00018809132,0.00019355558,0.0006381132],"category_scores_gemma":[0.0006064386,0.00017979486,0.00020608639,0.00042458985,0.00014364191,0.00019357313,0.00044267505,0.00019001304,0.000225024],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018520921,0.000055187178,0.95619917,0.000024115681,0.00006421257,0.00052921294,0.0005548648,0.0013394189,0.021623436,0.00017162408,0.00058780157,0.018665703],"study_design_scores_gemma":[0.000005504066,0.00004967393,0.9943988,0.000007858777,0.000015474858,0.00017895078,0.00023943544,0.0027969289,0.0012745033,0.00008370761,0.0009434379,0.0000056396775],"about_ca_topic_score_codex":0.0050958423,"about_ca_topic_score_gemma":0.009825174,"teacher_disagreement_score":0.0050958423,"about_ca_system_score_codex":0.00031955467,"about_ca_system_score_gemma":0.00014438716,"threshold_uncertainty_score":0.010132372},"labels":[],"label_agreement":null},{"id":"W3047514990","doi":"10.3847/1538-4357/aba903","title":"The Turbulent Gas Structure in the Centers of NGC 253 and the Milky Way","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council","keywords":"Milky Way; Velocity dispersion; Line (geometry); Hubble sequence; RADIUS; Interstellar medium; Turbulence; Galaxy","score_opus":0.0075241188719603795,"score_gpt":0.2130916788162731,"score_spread":0.20556755994431272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3047514990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99976224,0.000012852945,0.000022334187,0.0000033635624,3.443621e-7,4.4142348e-7,0.000038005503,0.0000035204075,0.00015701444],"genre_scores_gemma":[0.99982077,0.0000062295226,0.000033299853,0.0000016776945,7.175085e-7,5.4013947e-7,0.00010347487,0.0000016217936,0.000031729127],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992776,0.000006582017,0.0000041574663,0.000026209571,0.000010916099,0.000024312541],"domain_scores_gemma":[0.9995351,0.000046697383,0.00017386788,0.000032312048,0.00006412293,0.00014801329],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014111381,0.00011321095,0.00017990702,0.00087312603,0.00027114272,0.0005413528,0.00018309438,0.00013156702,0.00055137445],"category_scores_gemma":[0.00043871193,0.000083715684,0.00016671143,0.00059530634,0.00041599217,0.00024460987,0.0004093319,0.00009456933,0.000109955596],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037913883,0.000045962657,0.934064,0.00001827559,0.00007683809,0.0004191025,0.0012462245,0.002879996,0.054593,0.0012252519,0.00027963088,0.004772695],"study_design_scores_gemma":[0.0000041365715,0.000017708524,0.997203,0.0000034175357,0.000009407187,0.000041868112,0.00031011374,0.0011342164,0.0009822123,0.00010545365,0.00018362544,0.0000048617744],"about_ca_topic_score_codex":0.023431681,"about_ca_topic_score_gemma":0.018016601,"teacher_disagreement_score":0.023431681,"about_ca_system_score_codex":0.00074277853,"about_ca_system_score_gemma":0.0002085957,"threshold_uncertainty_score":0.046590626},"labels":[],"label_agreement":null},{"id":"W3047719262","doi":"10.3847/0004-637x/817/2/102","title":"ON SHOCKS DRIVEN BY HIGH-MASS PLANETS IN RADIATIVELY INEFFICIENT DISKS. II. THREE-DIMENSIONAL GLOBAL DISK SIMULATIONS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Planet; Physics; Astrobiology; Astrophysics","score_opus":0.007152695834883118,"score_gpt":0.23182639479070874,"score_spread":0.22467369895582562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3047719262","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98719597,0.00021317146,0.003060467,0.0004195594,0.000050555558,0.00006816956,0.001078027,0.00017496303,0.0077390913],"genre_scores_gemma":[0.99569255,0.00013297216,0.0019901032,0.00013835308,0.000025315985,0.000059614365,0.00077892136,0.00006137975,0.0011208581],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979013,0.000053833388,0.000010139506,0.000026255419,0.000033343258,0.00008631716],"domain_scores_gemma":[0.9987336,0.0006488153,0.00013625158,0.00007710668,0.0001433538,0.00026091174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053188443,0.0010100631,0.0012707035,0.00081539975,0.0009450363,0.0015921011,0.0017961569,0.0025151153,0.0034705112],"category_scores_gemma":[0.0024368265,0.0005571574,0.0012421646,0.00072280224,0.0016114096,0.0008647561,0.0014759459,0.0016753736,0.00033121326],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001816773,0.0001247532,0.005434909,0.000037879592,0.000046563153,0.00020999581,0.000053488522,0.99139786,0.00053245504,0.0010859554,0.00028360725,0.00061081763],"study_design_scores_gemma":[0.0000780155,0.00003888572,0.0014961238,0.0000066418743,0.0000086002665,0.000013230226,0.0000551768,0.99761486,0.00016034847,0.00039253285,0.00012703784,0.000008527628],"about_ca_topic_score_codex":0.031692043,"about_ca_topic_score_gemma":0.013761806,"teacher_disagreement_score":0.031692043,"about_ca_system_score_codex":0.0013483706,"about_ca_system_score_gemma":0.0008451685,"threshold_uncertainty_score":0.0630151},"labels":[],"label_agreement":null},{"id":"W3047745057","doi":"10.3847/1538-4357/abad37","title":"Revisiting the Magnetic Field of the L183 Starless Core","year":2020,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"James Clerk Maxwell Telescope; Physics; Astrophysics; Magnetic field; Polarization (electrochemistry); Star formation; Sky; Galaxy","score_opus":0.02204430297227885,"score_gpt":0.2663170982114369,"score_spread":0.24427279523915804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3047745057","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99916637,0.0000479327,0.00012608054,0.000022197626,0.0000013225684,0.0000019143135,0.00018383753,0.00001813235,0.00043223274],"genre_scores_gemma":[0.9995683,0.000019958747,0.00013564636,0.00001355068,0.0000040296927,0.0000012060644,0.00018449295,0.0000055330493,0.0000671762],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999591,0.0000021983565,0.0000013381374,0.000009830463,0.000012445205,0.000015129695],"domain_scores_gemma":[0.99984765,0.000011083287,0.000057024055,0.0000074500986,0.000018805416,0.000058017085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006328771,0.00018629983,0.00025267265,0.0006133456,0.00038375225,0.00036527595,0.0003053658,0.00018379105,0.0009470544],"category_scores_gemma":[0.00013299691,0.000111355585,0.00015499581,0.00044077367,0.00025546123,0.0001943115,0.00038308685,0.00027762385,0.00025281843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006102703,0.00010466803,0.5911185,0.00006540576,0.00005598139,0.0010915275,0.00060394325,0.0009930086,0.39357907,0.0003816447,0.00076509354,0.010630856],"study_design_scores_gemma":[0.000025462494,0.000053078664,0.9897384,0.000007942473,0.000012161936,0.00020363438,0.00015156207,0.0019161506,0.006798458,0.0001166922,0.00096968276,0.000006622055],"about_ca_topic_score_codex":0.010009927,"about_ca_topic_score_gemma":0.014197065,"teacher_disagreement_score":0.010009927,"about_ca_system_score_codex":0.00048338695,"about_ca_system_score_gemma":0.00018464384,"threshold_uncertainty_score":0.019903302},"labels":[],"label_agreement":null},{"id":"W3047831833","doi":"10.3847/1538-4357/abbdf6","title":"First Discovery of a Fast Radio Burst at 350 MHz by the GBNCC Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Compute Canada; Canarie; Office of Integrative Activities; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Fast radio burst; Green Bank Telescope; Pulsar; Source counts; Redshift; Galaxy; Flux (metallurgy); Radio telescope; Interstellar medium; Telescope","score_opus":0.017923310540336978,"score_gpt":0.28692761913153464,"score_spread":0.26900430859119767,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3047831833","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9885606,0.0006547268,0.0006164184,0.00028185057,0.000045896235,0.00003228055,0.004241538,0.00011347993,0.0054533393],"genre_scores_gemma":[0.99243027,0.00028174993,0.0014186645,0.0004268462,0.000058865964,0.000020787076,0.0042673773,0.000026093034,0.001069267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954766,0.000043394164,0.000016090164,0.00009546566,0.0001788582,0.00011845708],"domain_scores_gemma":[0.99851614,0.00014179516,0.00024337042,0.00013710413,0.00044220922,0.00051937794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050610764,0.000275102,0.00021456486,0.0015473223,0.0005632105,0.00078723516,0.00027258907,0.0003619296,0.0013933855],"category_scores_gemma":[0.0011437649,0.00019021987,0.00009052626,0.0011605937,0.00031953547,0.00017953105,0.000701,0.0003692524,0.0006288769],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023255355,0.000029755614,0.9495681,0.000047860332,0.000052314645,0.0006657483,0.00064518757,0.0001826537,0.017269935,0.00027225757,0.0069405017,0.024093235],"study_design_scores_gemma":[0.0000056054914,0.000022811599,0.9921221,0.000023548202,0.000012905294,0.00017335931,0.00011089706,0.00018435901,0.0007220667,0.00003091432,0.0065846415,0.000006635339],"about_ca_topic_score_codex":0.0653425,"about_ca_topic_score_gemma":0.12579262,"teacher_disagreement_score":0.0653425,"about_ca_system_score_codex":0.0010622734,"about_ca_system_score_gemma":0.0006136216,"threshold_uncertainty_score":0.1299243},"labels":[],"label_agreement":null},{"id":"W3048209480","doi":"10.3847/1538-4357/abad32","title":"13 yr of P Cygni Spectropolarimetry: Investigating Mass Loss through Hα, Periodicity, and Ellipticity","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced NMR Techniques and Applications","field":"Chemistry","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Astrophysics; Physics; Astronomy","score_opus":0.021571732666359575,"score_gpt":0.2738587652624553,"score_spread":0.2522870325960957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3048209480","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935953,0.00035388063,0.0022872637,0.00005966277,0.0000127638605,0.000014058322,0.0011095349,0.00007118268,0.0024963713],"genre_scores_gemma":[0.9963438,0.00013529998,0.0010939068,0.000042117816,0.000021062471,0.000008080089,0.001763308,0.000022202868,0.0005702177],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998652,0.000012129472,0.0000040688,0.000044997956,0.000045191828,0.000028416145],"domain_scores_gemma":[0.9997403,0.00003780138,0.00007153902,0.000031509862,0.00006506196,0.000053819716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053937885,0.00024432153,0.0002661884,0.0007207906,0.0005913007,0.0004021736,0.00019460818,0.0002956173,0.00053929945],"category_scores_gemma":[0.00038497077,0.00013913633,0.00018903271,0.0004892619,0.00029698428,0.00025472042,0.0005060553,0.0004960586,0.00031890094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037274678,0.00016600273,0.79903257,0.000035280373,0.00016266499,0.00042824022,0.0003728225,0.001795022,0.16577584,0.00033833855,0.0010133312,0.03050721],"study_design_scores_gemma":[0.000003309024,0.00007064918,0.98636395,0.0000038853123,0.000019687635,0.00019719629,0.000059256796,0.0014081732,0.009938591,0.00007583021,0.0018523562,0.000007095245],"about_ca_topic_score_codex":0.0061796275,"about_ca_topic_score_gemma":0.0074442457,"teacher_disagreement_score":0.0061796275,"about_ca_system_score_codex":0.0003327013,"about_ca_system_score_gemma":0.000157589,"threshold_uncertainty_score":0.012287319},"labels":[],"label_agreement":null},{"id":"W3048419233","doi":"10.3847/1538-4357/abc6fd","title":"SuperRAENN: A Semisupervised Supernova Photometric Classification Pipeline Trained on Pan-STARRS1 Medium-Deep Survey Supernovae","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Los Alamos National Laboratory; Science and Technology Facilities Council; Harvard Data Science Initiative, Harvard University; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Eötvös Loránd Tudományegyetem; European Commission; Johns Hopkins University; Harvard University; National Central University; Gordon and Betty Moore Foundation; Space Telescope Science Institute; Smithsonian Institution; Durham University; Alfred P. Sloan Foundation; FAS Division of Science, Harvard University; Horizon 2020 Framework Programme; Queen's University Belfast; National Aeronautics and Space Administration; National Science Foundation","keywords":"Light curve; Supernova; Galaxy; Large Synoptic Survey Telescope; Population; Type (biology); Autoencoder","score_opus":0.042614959060833,"score_gpt":0.2604540156637791,"score_spread":0.2178390566029461,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3048419233","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.57584006,0.0008980885,0.3699846,0.0006300318,0.000211062,0.00029576922,0.0047897687,0.041221537,0.0061291005],"genre_scores_gemma":[0.7809895,0.00013475883,0.19461396,0.00037439543,0.00007343051,0.00019852689,0.015360093,0.00046744788,0.0077878563],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99957794,0.000067669134,0.000023097464,0.00018013448,0.000079583464,0.000071584866],"domain_scores_gemma":[0.9991806,0.00019658402,0.000096669304,0.00019110081,0.00026407093,0.000070926326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010593393,0.0012409166,0.0006413822,0.00087207626,0.000366935,0.0005453195,0.0018317142,0.00084972684,0.0022448278],"category_scores_gemma":[0.0019035147,0.00043867363,0.0009092244,0.00040652812,0.00034717598,0.0008123616,0.0010896854,0.001130787,0.001601552],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052007206,0.00070217403,0.038506888,0.00018870356,0.0003973383,0.0002101189,0.00015276331,0.28481114,0.027693927,0.0015845299,0.02605404,0.61917824],"study_design_scores_gemma":[0.000016176416,0.000050248134,0.0027896685,0.000009246705,0.000013468461,0.000025841236,0.00001608998,0.99078697,0.004452915,0.0005912975,0.0012365775,0.000011429368],"about_ca_topic_score_codex":0.007856736,"about_ca_topic_score_gemma":0.012420475,"teacher_disagreement_score":0.007856736,"about_ca_system_score_codex":0.00057448,"about_ca_system_score_gemma":0.00091093266,"threshold_uncertainty_score":0.01562202},"labels":[],"label_agreement":null},{"id":"W3048647938","doi":"10.3847/1538-4357/ab9ec4","title":"Effects of Superthermal Plasmas on the Linear Growth of Multiband EMIC Waves","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Memorial University of Newfoundland","funders":"National Postdoctoral Program for Innovative Talents; National Natural Science Foundation of China","keywords":"Physics; Atomic physics; Plasma; Instability; Anisotropy; Cyclotron; Growth rate; Electron; Optics; Nuclear physics","score_opus":0.005517348030512307,"score_gpt":0.19285295239099204,"score_spread":0.18733560436047972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3048647938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961279,0.0002119826,0.002228918,0.000028698272,0.000005179128,0.0000061354226,0.000035100144,0.000046430123,0.001309658],"genre_scores_gemma":[0.99949324,0.000058776386,0.0002359438,0.0000050356184,0.0000022338604,0.000004153928,0.00001601472,0.000008745408,0.00017569591],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999038,0.00001252068,0.000004762232,0.000019781626,0.000028051749,0.000031057356],"domain_scores_gemma":[0.99942553,0.00028828182,0.00015079665,0.000033862638,0.000058521226,0.00004304866],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001350135,0.00025437045,0.0001387672,0.00021141558,0.00016244464,0.0002973523,0.0001566628,0.000110098284,0.0010312953],"category_scores_gemma":[0.00067110674,0.00013676716,0.00015190044,0.00014264048,0.00030585937,0.00023855148,0.00030883556,0.00023338561,0.00011058872],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031259595,0.000022718636,0.0034049044,0.00007177856,0.000014878741,0.00017440367,0.0001089985,0.0069611967,0.9838457,0.0004112876,0.00009316194,0.0045783753],"study_design_scores_gemma":[0.000019505676,0.00023517628,0.014640542,0.000008556481,0.000018803634,0.0001461608,0.0001214469,0.05528186,0.92867386,0.00026206276,0.0005790276,0.000012951814],"about_ca_topic_score_codex":0.0005439166,"about_ca_topic_score_gemma":0.0003952557,"teacher_disagreement_score":0.0010312953,"about_ca_system_score_codex":0.00019068384,"about_ca_system_score_gemma":0.000099604375,"threshold_uncertainty_score":0.0034500957},"labels":[],"label_agreement":null},{"id":"W3048751874","doi":"10.3847/1538-4357/abc42b","title":"Photometric Classification of 2315 Pan-STARRS1 Supernovae with Superphot","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Los Alamos National Laboratory; Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; Horizon 2020 Framework Programme; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; European Commission; Johns Hopkins University; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Smithsonian Institution; Durham University; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Supernova; Light curve; Classifier (UML); Python (programming language); Stars; Cosmology; Photometry (optics)","score_opus":0.02222188965630047,"score_gpt":0.2337601045346371,"score_spread":0.21153821487833663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3048751874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9599396,0.00013730892,0.016826645,0.00010335484,0.000043459866,0.00007280109,0.012441129,0.0053019086,0.0051337136],"genre_scores_gemma":[0.9508057,0.000087649794,0.018475685,0.0000575236,0.000032774024,0.0000422386,0.027688267,0.0003168104,0.0024932402],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995316,0.000047848946,0.00003850106,0.00011711835,0.00019516457,0.00006980204],"domain_scores_gemma":[0.9989089,0.00023101132,0.00021433912,0.00027327857,0.00023401588,0.00013845136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000928036,0.0003084248,0.00027759155,0.0020653896,0.0002757004,0.00065422757,0.0005016204,0.00024326926,0.0029588619],"category_scores_gemma":[0.0017890859,0.00013840142,0.00043978236,0.0011209489,0.00018164261,0.00048428023,0.00082409725,0.00028648894,0.0015802282],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052874204,0.00023122523,0.7255296,0.00017055708,0.00016268154,0.00033835942,0.0002841118,0.015505804,0.017644845,0.0010269325,0.019117845,0.21945935],"study_design_scores_gemma":[0.00003405854,0.00014191816,0.7873727,0.000039909253,0.000045871875,0.0004882694,0.00022494422,0.17744516,0.018505385,0.0012542241,0.014400033,0.000047471352],"about_ca_topic_score_codex":0.0039421064,"about_ca_topic_score_gemma":0.006572118,"teacher_disagreement_score":0.0039421064,"about_ca_system_score_codex":0.00038746154,"about_ca_system_score_gemma":0.00044498697,"threshold_uncertainty_score":0.009898365},"labels":[],"label_agreement":null},{"id":"W3048991045","doi":"10.3847/1538-4357/abafad","title":"Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds from ASAS-SN: Implications for Thorne–Żytkow Objects and Super-asymptotic Giant Branch Stars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration","keywords":"Stars; Large Magellanic Cloud; Supergiant; Small Magellanic Cloud; Asymptotic giant branch; Variable star; Red supergiant; Population; K-type main-sequence star","score_opus":0.014536127120372624,"score_gpt":0.2230702049149978,"score_spread":0.20853407779462518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3048991045","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995484,0.00008640359,0.00007610487,0.000013827462,0.0000021413152,0.000002695603,0.000054889264,0.000002397094,0.00021315846],"genre_scores_gemma":[0.99964404,0.000044276258,0.00010804347,0.0000066922994,0.000006353817,0.000001518548,0.00014199024,0.0000012135935,0.000045926616],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998517,0.000013079573,0.00001793538,0.000044866058,0.000036038447,0.000036471185],"domain_scores_gemma":[0.9992778,0.00008401714,0.00030368677,0.000052508887,0.000084261395,0.00019784489],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031617453,0.000287523,0.00032229113,0.0018183499,0.0008180474,0.0009813593,0.00036689654,0.00027969878,0.0009478602],"category_scores_gemma":[0.0005383129,0.00013645506,0.0002926825,0.0010935954,0.00071876403,0.00042457465,0.0007490869,0.00026582574,0.0002492083],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000032690987,0.000009060031,0.9941531,0.000008740001,0.000008992938,0.0001684428,0.000075417105,0.00007013148,0.0042716493,0.000048147045,0.000025962014,0.0011276945],"study_design_scores_gemma":[0.0000019469435,0.000026089618,0.9982622,0.0000054862016,0.00001079411,0.0003704804,0.00037266058,0.0003324831,0.00037287603,0.000094258445,0.00014819873,0.0000025207144],"about_ca_topic_score_codex":0.0021139062,"about_ca_topic_score_gemma":0.0041680136,"teacher_disagreement_score":0.0021139062,"about_ca_system_score_codex":0.00025388223,"about_ca_system_score_gemma":0.00025996327,"threshold_uncertainty_score":0.0042031407},"labels":[],"label_agreement":null},{"id":"W3049166091","doi":"10.3847/1538-4357/abafbe","title":"On the Spectral Evolution of Hot White Dwarf Stars. I. A Detailed Model Atmosphere Analysis of Hot White Dwarfs from SDSS DR12","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":313,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Stars; Sky; Stellar classification; Atmosphere (unit); Effective temperature; Main sequence; Stellar atmosphere; Spectral line","score_opus":0.013238693372278754,"score_gpt":0.21148545563866095,"score_spread":0.1982467622663822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3049166091","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99768615,0.00009099016,0.0010690514,0.000028159388,0.0000021345595,0.000004824045,0.00062412815,0.000092973976,0.00040166773],"genre_scores_gemma":[0.9972899,0.00006450197,0.0009752915,0.000010898251,0.0000042921433,0.000004869641,0.0014504365,0.000042810996,0.00015701602],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999219,0.000018935472,0.0000047674257,0.000027040569,0.000011330419,0.00001600804],"domain_scores_gemma":[0.99978715,0.00005656187,0.0000459551,0.000047650134,0.000022062499,0.000040607985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033113905,0.00040090084,0.0002975443,0.00053948886,0.00030195978,0.00043682274,0.0004254932,0.00030512252,0.00043348683],"category_scores_gemma":[0.00057363004,0.00020391907,0.0008160072,0.00034479058,0.00019248445,0.0003572258,0.0003343455,0.00017627994,0.00016255977],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021182687,0.0001421306,0.6387564,0.00008041223,0.0002888977,0.00028369165,0.00038771358,0.32820585,0.019983897,0.0019323429,0.00083221815,0.008894675],"study_design_scores_gemma":[0.00003170585,0.000074174866,0.4029078,0.000007161338,0.00006315386,0.00010058088,0.0001076746,0.5926859,0.0020520329,0.0007701893,0.0011769985,0.00002272496],"about_ca_topic_score_codex":0.018240338,"about_ca_topic_score_gemma":0.017068269,"teacher_disagreement_score":0.018240338,"about_ca_system_score_codex":0.00065586634,"about_ca_system_score_gemma":0.00022847595,"threshold_uncertainty_score":0.036268353},"labels":[],"label_agreement":null},{"id":"W3049746522","doi":"10.3847/1538-4357/abb77e","title":"The μ Tau Association: A 60 Myr Old Coeval Group at 150 pc from the Sun","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Espace pour la vie","funders":"","keywords":"Pleiades; Stars; Extinction (optical mineralogy); Population; myr; Group (periodic table); Hertzsprung–Russell diagram; Main sequence","score_opus":0.01184789545979989,"score_gpt":0.22168774111603812,"score_spread":0.20983984565623823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3049746522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917835,0.00004464035,0.0002115831,0.0000041172943,0.0000021667545,0.0000033125664,0.00008581354,0.000010731251,0.00045928848],"genre_scores_gemma":[0.9991916,0.00001777768,0.0002806396,0.0000041909075,0.0000049678397,0.0000018715319,0.00023680978,0.0000033836557,0.00025867348],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998958,0.000004947541,0.000005305796,0.000038312282,0.00002732301,0.000028228322],"domain_scores_gemma":[0.9996619,0.00002216547,0.000088945846,0.00003446735,0.00004004793,0.00015253753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013040645,0.0001679899,0.0002053011,0.0011467361,0.0005905564,0.00051104475,0.00022177133,0.0001416494,0.0013185819],"category_scores_gemma":[0.00022348943,0.00007736816,0.00022591077,0.00044628343,0.00018123104,0.00019137419,0.00059718906,0.00019605736,0.0005424509],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008730723,0.00003187919,0.9818024,0.000005562431,0.000021657444,0.0004302216,0.00019815633,0.00008680659,0.01032719,0.00010877223,0.00012786078,0.006772294],"study_design_scores_gemma":[0.000002806786,0.000042347045,0.9968984,0.0000016230664,0.000013088336,0.00069612503,0.00013029014,0.0004440356,0.0009593026,0.00004156986,0.0007681054,0.0000024128146],"about_ca_topic_score_codex":0.002177594,"about_ca_topic_score_gemma":0.00264204,"teacher_disagreement_score":0.002177594,"about_ca_system_score_codex":0.00013939157,"about_ca_system_score_gemma":0.0001111022,"threshold_uncertainty_score":0.0044110417},"labels":[],"label_agreement":null},{"id":"W3053282223","doi":"10.3847/1538-4357/abb08a","title":"Uncovering the Primary X-Ray Emission and Possible Starburst Component in the Polarized NLS1 Mrk 1239","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Emissivity; Galaxy; Ionization; Spectral index; Active galactic nucleus; Polarization (electrochemistry); Spectral line; Reflection (computer programming)","score_opus":0.014904933320276597,"score_gpt":0.22210716148628448,"score_spread":0.2072022281660079,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3053282223","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99883384,0.000062248655,0.00012796005,0.000032685166,0.000002564418,0.000002599923,0.00022568258,0.000018838538,0.0006935515],"genre_scores_gemma":[0.9989435,0.00003999893,0.00024368713,0.000016480499,0.0000051327934,0.0000028204838,0.0005086845,0.000008918585,0.00023079515],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999923,0.0000049476616,0.0000053276726,0.000024095289,0.000019089684,0.000023467124],"domain_scores_gemma":[0.9996859,0.000016819511,0.00014880407,0.000027810509,0.000034487643,0.00008627441],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014740591,0.00020888647,0.00028345254,0.0005772133,0.0005007018,0.0004955555,0.00029433717,0.00027196397,0.0013479706],"category_scores_gemma":[0.0002430029,0.000162122,0.00025825942,0.00041867414,0.00024908144,0.00019375111,0.0004396444,0.00028987744,0.0005373591],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046497537,0.00010316919,0.8190502,0.000058262747,0.00005641862,0.0027255702,0.0005116052,0.0006316926,0.1642503,0.00031486826,0.0006796934,0.011153249],"study_design_scores_gemma":[0.000005326162,0.00007516019,0.99305665,0.000008029313,0.000017985041,0.0014347695,0.00017825053,0.00079100154,0.0027848713,0.000062413295,0.0015786898,0.0000067351284],"about_ca_topic_score_codex":0.0029167647,"about_ca_topic_score_gemma":0.005435286,"teacher_disagreement_score":0.0029167647,"about_ca_system_score_codex":0.00043133847,"about_ca_system_score_gemma":0.000118385404,"threshold_uncertainty_score":0.005799532},"labels":[],"label_agreement":null},{"id":"W3057319655","doi":"10.3847/1538-4357/abb0e3","title":"A Machine-learning Approach to Integral Field Unit Spectroscopy Observations. I. H ii Region Kinematics","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Algorithm; Physics; Spectral line; Data cube; Convolutional neural network; Convolution (computer science); Artificial intelligence; Spectral resolution; Spectral density; Galaxy; Filter (signal processing); Field (mathematics); Computer science; Artificial neural network; Mathematics; Astrophysics; Telecommunications; Computer vision","score_opus":0.02631733663099023,"score_gpt":0.23059420776780587,"score_spread":0.20427687113681564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3057319655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5106546,0.0003648241,0.48206866,0.0004872284,0.00003276977,0.000063487285,0.00046306296,0.0019129284,0.003952475],"genre_scores_gemma":[0.9073639,0.000057187757,0.09114852,0.000045995977,0.000024279938,0.00002627331,0.0002856025,0.000060054233,0.000988343],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999136,0.000019801731,0.0000031203622,0.00003602614,0.000016789778,0.000010665599],"domain_scores_gemma":[0.9998041,0.000064458436,0.00004454311,0.000034044297,0.00003861357,0.000014216754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033325684,0.00038582386,0.00020484744,0.0006478535,0.00027315543,0.00040850043,0.00083824375,0.0005335868,0.0011098234],"category_scores_gemma":[0.0011066197,0.0003007124,0.00035111242,0.00053064304,0.0002603753,0.0006202792,0.0004158064,0.00043322763,0.00022301264],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007717931,0.00006305376,0.013630321,0.000036377915,0.00005261993,0.00008900202,0.000052855197,0.81402254,0.016624248,0.002426704,0.0009838411,0.1519413],"study_design_scores_gemma":[0.000002021989,0.0000059694607,0.0017971293,0.0000018170251,0.000001539741,0.0000072722255,0.000006094697,0.99588627,0.0013898739,0.0007293327,0.00016968517,0.0000029127893],"about_ca_topic_score_codex":0.013312835,"about_ca_topic_score_gemma":0.015220915,"teacher_disagreement_score":0.013312835,"about_ca_system_score_codex":0.0009884575,"about_ca_system_score_gemma":0.0003913478,"threshold_uncertainty_score":0.02647072},"labels":[],"label_agreement":null},{"id":"W3059615107","doi":"10.3847/1538-4357/abbe87","title":"Pair Plasma in Super-QED Magnetic Fields and the Hard X-Ray/Optical Emission of Magnetars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Magnetar; Bremsstrahlung; Scattering; Atomic physics; Plasma; Astrophysics; Annihilation; Compton scattering; Photon; Condensed matter physics; Neutron star; Nuclear physics; Quantum mechanics","score_opus":0.012217207028951136,"score_gpt":0.2634133883862544,"score_spread":0.25119618135730326,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3059615107","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99379694,0.00006778087,0.003511526,0.000031166997,0.000005401105,0.000005023564,0.000014034194,0.000057284877,0.0025108901],"genre_scores_gemma":[0.99948186,0.000011806634,0.00024976785,0.0000034694826,0.000004813758,0.0000027060094,0.00001139653,0.0000054542816,0.00022876705],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999325,0.000019604058,0.0000017562702,0.000010673871,0.000015413294,0.000020025134],"domain_scores_gemma":[0.9998951,0.000028679671,0.000028200855,0.000011712,0.000013952569,0.00002229846],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017891807,0.00026426357,0.00023257927,0.0003543497,0.00031566405,0.0004362163,0.00037224925,0.00019950587,0.0011110932],"category_scores_gemma":[0.00033105444,0.0001247209,0.00019247693,0.00018599063,0.000482289,0.00025728985,0.0005529309,0.00017095493,0.000114951676],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015663285,0.00027333945,0.052362632,0.00023482573,0.00029450204,0.005035363,0.0009445786,0.17504615,0.64643574,0.100838564,0.0010203035,0.015947627],"study_design_scores_gemma":[0.00035741372,0.0013629743,0.124577686,0.000020762925,0.00009846657,0.0016275784,0.00062468793,0.72912514,0.10981362,0.028939694,0.0033735544,0.00007851869],"about_ca_topic_score_codex":0.00034668218,"about_ca_topic_score_gemma":0.00013660268,"teacher_disagreement_score":0.0011110932,"about_ca_system_score_codex":0.00024284843,"about_ca_system_score_gemma":0.00007780512,"threshold_uncertainty_score":0.0037169456},"labels":[],"label_agreement":null},{"id":"W3068330295","doi":"10.3847/1538-4357/aba0b7","title":"An Exploration of Tensor Virial Equilibrium in Magnetized Molecular Cloud Cores","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Virial theorem; Physics; Statistical physics; Virial mass; Virial coefficient; Tensor (intrinsic definition); Population; Degeneracy (biology); Classical mechanics; Astrophysics; Quantum mechanics; Galaxy; Geometry; Mathematics","score_opus":0.02375858852046495,"score_gpt":0.2624957164304946,"score_spread":0.23873712791002963,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3068330295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.939757,0.000117612755,0.05006748,0.00031588232,0.000013723434,0.000047075635,0.00047004066,0.0003646805,0.008846466],"genre_scores_gemma":[0.989472,0.00003225926,0.009581079,0.00004071541,0.000008689644,0.000026096459,0.00027230242,0.000100093486,0.00046674703],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998684,0.000056023586,0.0000056702706,0.00001912658,0.000025655925,0.000025097122],"domain_scores_gemma":[0.9990508,0.0005034021,0.00013218896,0.000085957465,0.000116337054,0.000111340916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059498387,0.0003891866,0.0003562703,0.0006624625,0.0006848123,0.0012120573,0.00063839235,0.0004801798,0.0020654956],"category_scores_gemma":[0.0027420097,0.0003274385,0.00062068016,0.00037605417,0.0005269701,0.00088802574,0.00085934345,0.00037611084,0.00012947209],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000081264865,0.00005059897,0.014426189,0.000035623067,0.00004630244,0.00017680846,0.0001999412,0.94139725,0.00337148,0.03551555,0.0010741443,0.0036249086],"study_design_scores_gemma":[0.000009762523,0.000011175702,0.00066649436,0.0000038290796,0.000003080613,0.000022032964,0.000024895337,0.9930189,0.00036465612,0.005464685,0.00040507337,0.0000053745753],"about_ca_topic_score_codex":0.014289111,"about_ca_topic_score_gemma":0.011443135,"teacher_disagreement_score":0.014289111,"about_ca_system_score_codex":0.001163327,"about_ca_system_score_gemma":0.0007698419,"threshold_uncertainty_score":0.028411865},"labels":[],"label_agreement":null},{"id":"W3080078750","doi":"10.3847/1538-4357/abcaa4","title":"Multimessenger Gamma-Ray and Neutrino Coincidence Alerts Using HAWC and IceCube Subthreshold Data","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Institute for Computational and Data Sciences, Pennsylvania State University; Los Alamos National Laboratory; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Chiba University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Benemérita Universidad Autónoma de Puebla; Knut och Alice Wallenbergs Stiftelse; Coordinación de la Investigación Científica; Villum Fonden; National Research Foundation of Korea; Consejo Nacional de Ciencia y Tecnología; Fonds Wetenschappelijk Onderzoek; Chulalongkorn University; Marsden Fund; Bundesministerium für Bildung und Forschung; Danmarks Grundforskningsfond; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Laboratory Directed Research and Development; National Science Foundation; Belgian Federal Science Policy Office; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Deutsche Forschungsgemeinschaft; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Deutsches Elektronen-Synchrotron; Generalitat Valenciana; Pennsylvania State University; University of Oxford; Compute Canada; Marquette University; Vetenskapsrådet; U.S. Department of Energy; University of Wisconsin-Madison; National Research Foundation; Michigan State University","keywords":"Physics; Cherenkov radiation; Neutrino; Observatory; Coincidence; Cosmic ray; Gamma ray; COSMIC cancer database; Astronomy; Astrophysics; Detector; Particle physics","score_opus":0.031164962452990268,"score_gpt":0.26397018710049786,"score_spread":0.23280522464750758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3080078750","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95682704,0.00015150732,0.012156321,0.00013319694,0.000074023075,0.00012579386,0.021699786,0.0020617566,0.006770498],"genre_scores_gemma":[0.9266568,0.000061519415,0.028274573,0.000037109432,0.000037944268,0.000087973196,0.043016847,0.00035962395,0.001467668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991804,0.00013365818,0.000035274246,0.00026477673,0.00027002007,0.00011587553],"domain_scores_gemma":[0.9986009,0.00034467038,0.0002025207,0.0003226552,0.0003949851,0.00013425767],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001259258,0.0005581995,0.0004680179,0.0017749361,0.00045301838,0.0012268651,0.0006184213,0.00031824975,0.0021475304],"category_scores_gemma":[0.0029764345,0.0002055816,0.00039795256,0.0019678832,0.00031273326,0.00064280804,0.0010434103,0.00045126586,0.00059148594],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021829018,0.00042345436,0.68255067,0.0002338011,0.0005665544,0.0010795018,0.00077223225,0.14034082,0.025911208,0.004422751,0.023729289,0.117786765],"study_design_scores_gemma":[0.00017623388,0.00024575542,0.5098763,0.00007004844,0.00013606685,0.00034036723,0.0006577292,0.41728508,0.03646477,0.0039091404,0.030685682,0.00015284687],"about_ca_topic_score_codex":0.023588149,"about_ca_topic_score_gemma":0.03726035,"teacher_disagreement_score":0.023588149,"about_ca_system_score_codex":0.0008153135,"about_ca_system_score_gemma":0.0007442421,"threshold_uncertainty_score":0.046901703},"labels":[],"label_agreement":null},{"id":"W3080761822","doi":"10.3847/1538-4357/ac0bbc","title":"Probing Galaxy Evolution in Massive Clusters Using ACT and DES: Splashback as a Cosmic Clock","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"SLAC National Accelerator Laboratory; Integrated Electronics Engineering Center, Binghamton University; European Regional Development Fund; Leibniz-Gemeinschaft; Science and Technology Facilities Council; Kavli Institute for Cosmological Physics, University of Chicago; Office of Science; University of Illinois at Urbana-Champaign; University of California, Santa Cruz; Inyuvesi Yakwazulu-Natali; Generalitat de Catalunya; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Center for Cosmology and Astroparticle Physics, Ohio State University; University of Sussex; High Energy Physics; Deutsche Forschungsgemeinschaft; Argonne National Laboratory; Centres de Recerca de Catalunya; Fermilab; National Science Foundation; Compute Canada; University of Portsmouth; Ohio State University; Comisión Nacional de Investigación Científica y Tecnológica; University College London; National Aeronautics and Space Administration; Lawrence Berkeley National Laboratory; Financiadora de Estudos e Projetos; University of Pennsylvania; Stanford Research Computing Center, Stanford University; Ministerio de Ciencia e Innovación; European Commission; U.S. Department of Energy; Princeton University; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministerio de Economía y Competitividad; Government of Ontario; University of Toronto; Institut de Física d'Altes Energies; Eidgenössische Technische Hochschule Zürich; National Centre for Supercomputing Applications","keywords":"Physics; COSMIC cancer database; Galaxy; Astronomy; Astrophysics; Galaxy cluster; Galaxy formation and evolution","score_opus":0.010100963627139331,"score_gpt":0.22712756185795516,"score_spread":0.21702659823081583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3080761822","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952539,0.00003711466,0.0013266178,0.00006151019,0.000008278328,0.0000072767284,0.0015110279,0.00030894758,0.0014852739],"genre_scores_gemma":[0.9970395,0.00001507288,0.0010567117,0.000018646439,0.0000065413096,0.0000060356324,0.0015017582,0.00003805288,0.00031753362],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997625,0.000056255616,0.0000076204087,0.00007164453,0.000065532,0.000036469322],"domain_scores_gemma":[0.99883443,0.00019938058,0.00024682962,0.00027164386,0.00014618218,0.00030150765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046616746,0.00030046792,0.00027733998,0.0006715546,0.0002153443,0.0005876088,0.00043743636,0.00023600346,0.001859785],"category_scores_gemma":[0.0020768761,0.00025602887,0.00031022166,0.00071919267,0.00028956335,0.00044452868,0.00049964746,0.00032769423,0.00039828083],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010811673,0.00015481019,0.91214854,0.000045711204,0.00023069729,0.00014566473,0.00035536676,0.047099266,0.011678083,0.0032020854,0.0047865524,0.019071989],"study_design_scores_gemma":[0.000040005292,0.00009532991,0.8733795,0.0000071389377,0.000038667185,0.00007938449,0.00009842094,0.11726885,0.0055104126,0.00092875044,0.002521784,0.000031710777],"about_ca_topic_score_codex":0.008657775,"about_ca_topic_score_gemma":0.009509996,"teacher_disagreement_score":0.008657775,"about_ca_system_score_codex":0.00064972515,"about_ca_system_score_gemma":0.00018695254,"threshold_uncertainty_score":0.017214775},"labels":[],"label_agreement":null},{"id":"W3080945812","doi":"10.3847/1538-4357/abb0e5","title":"New Calculations of Stark-broadened Profiles for Neutral Helium Lines Using Computer Simulations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Laser-induced spectroscopy and plasma","field":"Engineering","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Helium; Electron; Ion; Charged particle; Electron density; Debye; Neutral particle; Core (optical fiber)","score_opus":0.02835688767191398,"score_gpt":0.25928489018157,"score_spread":0.23092800250965606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3080945812","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8763568,0.00031097123,0.095134236,0.00043313697,0.000117102165,0.00017410656,0.00068358984,0.00083082274,0.025959294],"genre_scores_gemma":[0.97167844,0.0001211962,0.025266638,0.00007362266,0.000017625596,0.0001672798,0.0003275787,0.00015948922,0.0021881212],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997273,0.00009188845,0.000011438508,0.000021266955,0.00009779739,0.000050187282],"domain_scores_gemma":[0.9977049,0.0013362172,0.00012799376,0.00016730829,0.0005272243,0.00013630169],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007656533,0.00051774847,0.0008236074,0.00087240036,0.0008978722,0.000942651,0.0012212814,0.0011186709,0.0028002837],"category_scores_gemma":[0.004294973,0.00046958218,0.000521034,0.0013816304,0.000873351,0.00078102475,0.0006186627,0.0007903463,0.00023637347],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005169147,0.00003847598,0.0007097925,0.000023190458,0.00001624707,0.000055019667,0.00004288721,0.99371654,0.00075070624,0.0030709098,0.00020319466,0.0013213569],"study_design_scores_gemma":[0.000019890185,0.000011816992,0.00014455171,0.000003637757,0.0000038293606,0.0000046724067,0.000013714056,0.99844486,0.00044124818,0.0006844527,0.00022244758,0.0000049193086],"about_ca_topic_score_codex":0.013432968,"about_ca_topic_score_gemma":0.008662266,"teacher_disagreement_score":0.013432968,"about_ca_system_score_codex":0.0015356037,"about_ca_system_score_gemma":0.0013466785,"threshold_uncertainty_score":0.026709557},"labels":[],"label_agreement":null},{"id":"W3081572918","doi":"10.3847/1538-4357/ac1596","title":"CMB-S4: Forecasting Constraints on Primordial Gravitational Waves","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":261,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; Simon Fraser University; University of British Columbia; McGill University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Berkeley National Laboratory; SLAC National Accelerator Laboratory; Fermilab; Science and Technology Facilities Council; Office of Science; Nuclear Safety and Security Commission; Agence Nationale de la Recherche; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Argonne National Laboratory; U.S. Department of Energy; European Commission; National Energy Research Scientific Computing Center; Canadian Institute for Advanced Research; Basic Energy Sciences; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Harvard University; National Science Foundation","keywords":"Cosmic microwave background; Gravitational wave; Physics; Gravitational lens; Gravitation; Astrophysics; Sky; Polarization (electrochemistry); Astronomy; Redshift; Optics; Galaxy","score_opus":0.015929888999532883,"score_gpt":0.2498183196093684,"score_spread":0.23388843060983552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3081572918","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.65654755,0.00022394852,0.31112894,0.002288982,0.00010888581,0.00024662897,0.005785436,0.006427186,0.017242415],"genre_scores_gemma":[0.91525793,0.00005582802,0.080722496,0.00009152281,0.00002864578,0.0001081525,0.0026739424,0.0003534783,0.0007079558],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991503,0.00042999783,0.000018232004,0.00009837891,0.00023197771,0.00007109509],"domain_scores_gemma":[0.9966568,0.0013694831,0.000411293,0.0005894856,0.0006244759,0.0003484145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0059796358,0.00090865366,0.00041083564,0.00078928773,0.0004658927,0.001150443,0.0015236165,0.00083051424,0.0022261462],"category_scores_gemma":[0.011506213,0.0004708374,0.0005852451,0.0006267094,0.00074798125,0.0011806593,0.0014084359,0.0011819386,0.00064437644],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061137846,0.00008946264,0.031029092,0.00008824911,0.00011398685,0.000071317336,0.00012616375,0.9036792,0.00790249,0.017310921,0.00530455,0.03367325],"study_design_scores_gemma":[0.00006300726,0.000054104778,0.0056972285,0.000009702228,0.000008964857,0.000007517304,0.00001933346,0.98202354,0.0035233,0.0070437454,0.0015245709,0.000025104899],"about_ca_topic_score_codex":0.011801102,"about_ca_topic_score_gemma":0.0065024737,"teacher_disagreement_score":0.011801102,"about_ca_system_score_codex":0.0011544796,"about_ca_system_score_gemma":0.0015319765,"threshold_uncertainty_score":0.03162372},"labels":[],"label_agreement":null},{"id":"W3081861499","doi":"10.3847/1538-4357/abce58","title":"The SAGA Survey. II. Building a Statistical Sample of Satellite Systems around Milky Way–like Galaxies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":183,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; High Energy Physics; Division of Astronomical Sciences; Japan Science and Technology Agency; Integrated Electronics Engineering Center, Binghamton University; Japan Society for the Promotion of Science; Leibniz-Gemeinschaft; Stanford Research Computing Center, Stanford University; Smithsonian Astrophysical Observatory; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; University of Colorado Boulder; Office of Science; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Space Telescope Science Institute; University of Sussex; Institut de Física d'Altes Energies; Yale University; U.S. Department of Energy; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Science and Technology Facilities Council; York University; Ministério da Ciência, Tecnologia e Inovação; University of Illinois at Urbana-Champaign; Cabinet Office, Government of Japan; Deutsche Forschungsgemeinschaft; Chinese Academy of Sciences; Academia Sinica; European Southern Observatory; Ministry of Education, Culture, Sports, Science and Technology; University of Oxford; Flatiron Health; University of Chicago; National Energy Research Scientific Computing Center; Instituto de Astrofísica de Canarias; Heising-Simons Foundation; Universidad Nacional Autónoma de México; University of Notre Dame; Carnegie Mellon University; University of Pittsburgh; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Vanderbilt University; High Energy Accelerator Research Organization; Ohio State University; Aspen Center for Physics; Carnegie Institution of Washington; University of Portsmouth; New Mexico State University; University of Utah; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Toray Science Foundation; National Geographic Society; Smithsonian Institution; University of Pennsylvania; University College London; National Aeronautics and Space Administration; California Institute of Technology; National Astronomical Observatory of Japan; National Science Foundation","keywords":"Milky Way; Galaxy; Satellite galaxy; Local Group; Satellite; Redshift; Luminosity; Galaxy formation and evolution; RADIUS","score_opus":0.015868538351485887,"score_gpt":0.2354351427986415,"score_spread":0.21956660444715562,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3081861499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9865986,0.00008437633,0.0013174859,0.00005038062,0.0000026741418,0.000037705246,0.011043748,0.00008847886,0.00077643024],"genre_scores_gemma":[0.96284646,0.00006507145,0.0023303127,0.000033697732,0.00001210555,0.000043045053,0.034213156,0.00004073438,0.00041546475],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99946374,0.00015606107,0.000032134492,0.00015937422,0.00011811674,0.00007064315],"domain_scores_gemma":[0.9981893,0.00028250227,0.00048551423,0.000422654,0.0003206948,0.00029934235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096270087,0.00023766089,0.0002670043,0.0020442156,0.00029387392,0.0006084771,0.00055194256,0.00024062909,0.0010991289],"category_scores_gemma":[0.00201584,0.00028347605,0.00045054549,0.0016642031,0.0002383214,0.00042223648,0.00091922295,0.00026594996,0.00081291876],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005466192,0.000030584695,0.9871272,0.000016869657,0.000100722915,0.00004787549,0.00014401482,0.0015055966,0.0012851611,0.00024453862,0.0016108544,0.007831863],"study_design_scores_gemma":[0.000011043092,0.00003824769,0.9934928,0.0000036126792,0.000019376832,0.00005629987,0.00014375497,0.0033858023,0.00026458467,0.0001084299,0.002470784,0.0000052911555],"about_ca_topic_score_codex":0.025543464,"about_ca_topic_score_gemma":0.024612464,"teacher_disagreement_score":0.025543464,"about_ca_system_score_codex":0.00039392334,"about_ca_system_score_gemma":0.00033424227,"threshold_uncertainty_score":0.050789535},"labels":[],"label_agreement":null},{"id":"W3081976656","doi":"10.3847/1538-4357/aba52f","title":"Dissecting the Global Cold Dust Properties and Possible Submillimeter Excess of 13 Nearby Spiral Galaxies from the NGLS","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Spiral galaxy; Galaxy; Black-body radiation; Astronomy; Luminous infrared galaxy; Spectral energy distribution; Luminosity; Metallicity; Submillimeter Array; Star formation; Radiation","score_opus":0.01937089758662755,"score_gpt":0.21062663962831857,"score_spread":0.19125574204169102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3081976656","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995857,0.000017811508,0.00006921589,0.000003236875,2.3779805e-7,0.0000011979671,0.00016558835,0.0000055011446,0.00015160805],"genre_scores_gemma":[0.99913234,0.000012713302,0.000109861045,0.0000034669695,0.0000010034396,0.0000020191549,0.0006368993,0.00000235402,0.00009932514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998926,0.00001276286,0.000007717846,0.000029703984,0.000026714077,0.000030479468],"domain_scores_gemma":[0.9996024,0.00004404384,0.00011136627,0.00006140395,0.00006396283,0.000116770294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026721976,0.00021385023,0.000265519,0.0014243034,0.00030726782,0.00040598982,0.00019517158,0.00016711616,0.0010002947],"category_scores_gemma":[0.00039466872,0.000121133,0.00027598577,0.0009430957,0.00019457273,0.00017372808,0.00042746597,0.000087653825,0.00029671003],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004540719,0.000012374794,0.9931815,0.0000058419337,0.000026277186,0.00006367828,0.00015083251,0.00021381983,0.004009474,0.000032314492,0.000054845335,0.002203689],"study_design_scores_gemma":[0.0000020357538,0.000014597749,0.9987424,0.0000014105801,0.00001028154,0.00004786459,0.000108552005,0.00042655325,0.00040348177,0.000022689119,0.00021841637,0.0000016506078],"about_ca_topic_score_codex":0.009202094,"about_ca_topic_score_gemma":0.01803832,"teacher_disagreement_score":0.009202094,"about_ca_system_score_codex":0.0003882489,"about_ca_system_score_gemma":0.00012971305,"threshold_uncertainty_score":0.018297076},"labels":[],"label_agreement":null},{"id":"W3082103229","doi":"10.3847/1538-4357/abb5af","title":"CANDELS Meets GSWLC: Evolution of the Relationship between Morphology and Star Formation Since z = 2","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Redshift; Star formation; Galaxy; Coalescence (physics); COSMIC cancer database; Morphology (biology); Grism; Spheroid","score_opus":0.027587560788923757,"score_gpt":0.24831134872005725,"score_spread":0.2207237879311335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3082103229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951479,0.00013508412,0.000112154754,0.00009260505,0.0000041823946,0.0000031463035,0.0028483006,0.000047147347,0.0016095792],"genre_scores_gemma":[0.9960675,0.000034682864,0.0001013558,0.000023266635,0.000006556607,0.0000021208093,0.0032484455,0.000012762677,0.0005032918],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999728,0.000024629495,0.000010750577,0.00010945737,0.000051461036,0.000075666925],"domain_scores_gemma":[0.99758935,0.00031573785,0.00062593713,0.00022935962,0.00044588937,0.00079384743],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006305333,0.00018265478,0.00023368263,0.00198651,0.0003683067,0.001391566,0.00042318666,0.00029839255,0.0036044766],"category_scores_gemma":[0.002516998,0.00014933832,0.00027599235,0.0013646069,0.00027379917,0.00065359066,0.0009383641,0.00036916515,0.00085704855],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042973195,0.000007303377,0.995236,0.0000056326385,0.000025153473,0.000027602193,0.00006897894,0.000201805,0.00048271226,0.00010569021,0.000589301,0.0032069332],"study_design_scores_gemma":[9.791128e-7,0.0000058847804,0.99945027,0.0000012715861,0.00000269185,0.000012593699,0.00005484301,0.00015283967,0.00008397997,0.000014740286,0.00021823813,0.0000016711655],"about_ca_topic_score_codex":0.03574517,"about_ca_topic_score_gemma":0.038470283,"teacher_disagreement_score":0.03574517,"about_ca_system_score_codex":0.0006531286,"about_ca_system_score_gemma":0.00035594692,"threshold_uncertainty_score":0.07107425},"labels":[],"label_agreement":null},{"id":"W3082140032","doi":"10.1086/519232","title":"The Disk and Extraplanar Regions of NGC 2403","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Red supergiant; Stars; Surface brightness; Galaxy; Astronomy; Metallicity; Spiral galaxy; RADIUS; Brightness; Supergiant","score_opus":0.007304412484717496,"score_gpt":0.2154050922557211,"score_spread":0.2081006797710036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3082140032","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.71630085,0.003873105,0.00065603066,0.015617812,0.016641067,0.0002823254,0.009234789,0.0009863653,0.23640753],"genre_scores_gemma":[0.7650536,0.002146559,0.00084168167,0.0014876589,0.006562729,0.00006023855,0.008186113,0.00042995144,0.21523154],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99942917,0.000049041028,0.000032250562,0.00008542285,0.00030847912,0.0000956116],"domain_scores_gemma":[0.9914601,0.0005171007,0.0005316841,0.0004056504,0.005828325,0.0012570666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060376263,0.00026767058,0.0004261136,0.0021530576,0.0014639895,0.0013516588,0.00054195325,0.0010720488,0.056756906],"category_scores_gemma":[0.005286813,0.00015373543,0.00018564516,0.0011028916,0.00044956157,0.0006998019,0.0006885953,0.00031576998,0.012063748],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015303514,0.00017421738,0.20357236,0.0013640939,0.00008076002,0.009881382,0.0018602709,0.0007093898,0.045661118,0.0029382757,0.5252941,0.20693369],"study_design_scores_gemma":[0.000101588106,0.00017064039,0.6422634,0.00012750829,0.000045750065,0.0016192984,0.001281213,0.00048605664,0.003897064,0.000904619,0.3490586,0.00004420252],"about_ca_topic_score_codex":0.0070617525,"about_ca_topic_score_gemma":0.011285519,"teacher_disagreement_score":0.056756906,"about_ca_system_score_codex":0.000623766,"about_ca_system_score_gemma":0.0009364166,"threshold_uncertainty_score":0.18987077},"labels":[],"label_agreement":null},{"id":"W3082181328","doi":"10.3847/1538-4357/abbd98","title":"The Zwicky Transient Facility Bright Transient Survey. II. A Public Statistical Sample for Exploring Supernova Demographics*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":264,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Benoziyo Endowment Fund for the Advancement of Science; Eötvös Loránd Tudományegyetem; Stockholms Universitet; National Central University; National Science Foundation; Liverpool John Moores University; Indian Institute of Technology Bombay; Weizmann Institute of Science; Israel Science Foundation; Gordon and Betty Moore Foundation; Queen's University Belfast; Aspen Center for Physics; Washington Research Foundation; Queen's University; Lawrence Berkeley National Laboratory; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Texas Tech University; San Diego State University; Northwestern University; U.S. Department of Energy; Smithsonian Institution; Los Alamos National Laboratory; University of Washington; Alfred P. Sloan Foundation; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Space Telescope Science Institute; W. M. Keck Foundation; Yuhan","keywords":"Supernova; Galaxy; Luminosity; Transient (computer programming); Sky; Gravitational microlensing; Light curve; Absolute magnitude","score_opus":0.06695724485617019,"score_gpt":0.2533309509460257,"score_spread":0.1863737060898555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3082181328","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5903561,0.00034638564,0.0027480535,0.00035373645,0.000017118271,0.0004946942,0.39599758,0.00045698034,0.009229385],"genre_scores_gemma":[0.38708505,0.0003535151,0.0034512526,0.00015650982,0.0000448994,0.0008605653,0.6012131,0.00027328162,0.0065618088],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994394,0.000044809465,0.000054694287,0.00012677701,0.0001823762,0.00015188556],"domain_scores_gemma":[0.99638534,0.00031847673,0.0017246993,0.00052714755,0.0005500088,0.0004943559],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010213946,0.00032090317,0.00024273223,0.005143755,0.00041128194,0.00073231076,0.00065331225,0.00021984498,0.009131883],"category_scores_gemma":[0.0033117551,0.0002631259,0.0002306637,0.00460503,0.00022766812,0.00081009744,0.0013821864,0.0002719082,0.0033567061],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020959832,0.000050459843,0.92375165,0.000062096566,0.00005265822,0.000090402806,0.00024930018,0.00035759402,0.0021479563,0.00095440197,0.044614203,0.02745979],"study_design_scores_gemma":[0.000031349926,0.000027680198,0.9783619,0.000024924357,0.00001258207,0.00012313032,0.00017709153,0.0005440109,0.0005108728,0.00014112936,0.02003498,0.000010306419],"about_ca_topic_score_codex":0.05184295,"about_ca_topic_score_gemma":0.0710808,"teacher_disagreement_score":0.05184295,"about_ca_system_score_codex":0.00087971566,"about_ca_system_score_gemma":0.0010979003,"threshold_uncertainty_score":0.10308242},"labels":[],"label_agreement":null},{"id":"W3082723280","doi":"10.3847/1538-4357/abc627","title":"Toward Extremely Precise Radial Velocities. II. A Tool for Using Multivariate Gaussian Processes to Model Stellar Activity","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"","keywords":"Univariate; Gaussian process; Doppler effect; Covariance; Radial velocity; Multivariate statistics; Series (stratigraphy); Covariance function; Gaussian","score_opus":0.05802176181858309,"score_gpt":0.2689287820010402,"score_spread":0.2109070201824571,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3082723280","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0042545972,0.000018576182,0.99264175,0.000048554644,0.000010249892,0.0000075586254,0.00009328598,0.0026085654,0.00031688917],"genre_scores_gemma":[0.21198559,0.00014660707,0.7827349,0.00012419347,0.000039257757,0.000121051504,0.0005007331,0.0020850166,0.0022626966],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996106,0.00012592565,0.000021361384,0.000089947134,0.00012383818,0.000028353641],"domain_scores_gemma":[0.9984529,0.0008607098,0.00023806911,0.00025085924,0.00014690068,0.000050612536],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014714894,0.00061587326,0.00030825136,0.00064754795,0.0002988062,0.0009366294,0.0011485049,0.00074542384,0.0037801617],"category_scores_gemma":[0.00697215,0.0005641462,0.00076767785,0.000636348,0.00051429047,0.0013058479,0.0012377942,0.0013900435,0.0016966857],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011296056,0.00007783823,0.006181305,0.00013102255,0.00009243888,0.00018784121,0.00024312561,0.75493795,0.016936278,0.062440544,0.006976276,0.15168238],"study_design_scores_gemma":[0.000010050829,0.0000103233915,0.0004739664,0.0000061916635,0.000003983303,0.00004035955,0.000008178336,0.98295045,0.0022198053,0.010689446,0.003573008,0.000014309542],"about_ca_topic_score_codex":0.006261764,"about_ca_topic_score_gemma":0.0050962097,"teacher_disagreement_score":0.006261764,"about_ca_system_score_codex":0.00044217822,"about_ca_system_score_gemma":0.0007462107,"threshold_uncertainty_score":0.0126459},"labels":[],"label_agreement":null},{"id":"W3082907167","doi":"10.3847/1538-4357/abdfd2","title":"Observing the Stellar Halo of Andromeda in Cosmological Simulations: The AURIGA2PANDAS Pipeline","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; Centre National de la Recherche Scientifique; Comisión Nacional de Investigación Científica y Tecnológica; Ministerio de Ciencia e Innovación; Science and Technology Facilities Council; Max-Planck-Gesellschaft","keywords":"Halo; Milky Way; Galaxy; Andromeda; Galactic halo; Star formation; Accretion (finance); Stars; Stellar density; Stellar mass","score_opus":0.01663433591421424,"score_gpt":0.23723889088783184,"score_spread":0.2206045549736176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3082907167","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8795974,0.00052382663,0.026775531,0.0006783961,0.00022300985,0.00021193492,0.020742439,0.053117376,0.018130086],"genre_scores_gemma":[0.922807,0.0002458301,0.048984013,0.00038916492,0.000054190892,0.00018014446,0.019245042,0.005583264,0.002511246],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99977106,0.00007532688,0.000009800179,0.000048782684,0.000050337934,0.00004479557],"domain_scores_gemma":[0.99928635,0.00021493789,0.000042696996,0.0002191506,0.00007848201,0.00015842557],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081479625,0.00079440867,0.00066869025,0.00043364597,0.00052958674,0.000998714,0.0017522424,0.0007056379,0.0035719494],"category_scores_gemma":[0.0023738174,0.00063690165,0.00091665256,0.000468867,0.0003638073,0.000660203,0.001270652,0.000974113,0.001276783],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014038348,0.00051444623,0.09921219,0.0005582847,0.0016624433,0.000810064,0.0015347839,0.7953123,0.014665513,0.011251433,0.044759344,0.028315427],"study_design_scores_gemma":[0.00072277384,0.00019010066,0.027198987,0.00005914016,0.00019893824,0.00021132822,0.00030085593,0.9167517,0.007331355,0.006252248,0.04061608,0.00016640073],"about_ca_topic_score_codex":0.025205422,"about_ca_topic_score_gemma":0.02751634,"teacher_disagreement_score":0.025205422,"about_ca_system_score_codex":0.00062666915,"about_ca_system_score_gemma":0.0007262317,"threshold_uncertainty_score":0.050117433},"labels":[],"label_agreement":null},{"id":"W3083030628","doi":"10.3847/1538-4357/abb372","title":"Spectroscopic Detection of the Pre-White Dwarf Companion of Regulus","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"National Science Foundation","keywords":"Physics; White dwarf; Astrophysics; Orbital inclination; Spectral line; RADIUS; Orbital elements; Effective temperature; Binary star; Orbital period; Stars; Binary number; Astronomy","score_opus":0.009896784603191211,"score_gpt":0.21383141867349179,"score_spread":0.20393463407030057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3083030628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937266,0.00001569554,0.0001805997,0.0000034387829,8.1883996e-7,0.0000012542866,0.000035271787,0.000012917635,0.0003772677],"genre_scores_gemma":[0.99943703,0.0000066112652,0.0002971857,0.0000037411191,0.0000010821019,9.0858833e-7,0.00012599773,0.000003626055,0.00012377524],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998889,0.000012325394,0.0000066995262,0.0000348775,0.000037665206,0.000019585881],"domain_scores_gemma":[0.9996953,0.000060501487,0.00008001497,0.0000459564,0.000050851348,0.0000674387],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023645777,0.00019663358,0.00017031647,0.00055589806,0.00033181818,0.0003044083,0.00022043352,0.00023395885,0.0007104256],"category_scores_gemma":[0.00044277127,0.00014773263,0.00013101881,0.00019621331,0.00022179374,0.00013493022,0.00027479322,0.00015399173,0.00023007943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032383783,0.000094051764,0.66044635,0.000040341634,0.000045435416,0.00093145535,0.00031707616,0.0010013825,0.3274029,0.00031091578,0.00017809308,0.008908125],"study_design_scores_gemma":[0.0000066580983,0.00024822145,0.9583427,0.000005422554,0.000020520398,0.0011633605,0.00013782954,0.003930025,0.03549293,0.00011216196,0.00053321966,0.0000070740775],"about_ca_topic_score_codex":0.0011917526,"about_ca_topic_score_gemma":0.0019814568,"teacher_disagreement_score":0.0011917526,"about_ca_system_score_codex":0.00014731105,"about_ca_system_score_gemma":0.00008725236,"threshold_uncertainty_score":0.002376616},"labels":[],"label_agreement":null},{"id":"W3083369691","doi":"10.3847/1538-4357/abb5a4","title":"The Dynamics, Destruction, and Survival of Supernova-formed Dust Grains","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"National Aeronautics and Space Administration","keywords":"Supernova; Ejecta; Interstellar medium; Cosmic dust; Stars; Interplanetary dust cloud; Dust lane; Asymptotic giant branch; Presolar grains","score_opus":0.011888423083278274,"score_gpt":0.22610993939558124,"score_spread":0.21422151631230296,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3083369691","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99821484,0.000055256707,0.0008153233,0.000014219802,0.0000034589268,0.0000032238222,0.000058354366,0.000025993835,0.00080936897],"genre_scores_gemma":[0.99934846,0.000023668697,0.00028685117,0.0000035863338,0.0000013400804,0.000002326226,0.00006695832,0.00000719659,0.00025956077],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999529,0.0000039805136,0.000002930608,0.000013011399,0.00001063791,0.00001649992],"domain_scores_gemma":[0.99979836,0.00005353034,0.000054134336,0.000017527427,0.000024302788,0.000052144755],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014684726,0.00021090599,0.00021113193,0.00029208988,0.00042479206,0.0006607472,0.00037981645,0.00029154847,0.0008388186],"category_scores_gemma":[0.00052236643,0.0002308474,0.00038473782,0.00015262027,0.0004266255,0.0002916694,0.000263605,0.00026420612,0.00015096995],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043715668,0.00019437859,0.30520684,0.000074984804,0.0002439135,0.0007438612,0.00022136937,0.55206615,0.12731022,0.006522906,0.00051506504,0.006463111],"study_design_scores_gemma":[0.000046951176,0.00013461857,0.10068214,0.0000056988447,0.000038654438,0.0002285318,0.00013034944,0.8730842,0.023906065,0.00094137946,0.0007745811,0.000026820282],"about_ca_topic_score_codex":0.0112728,"about_ca_topic_score_gemma":0.0045456565,"teacher_disagreement_score":0.0112728,"about_ca_system_score_codex":0.0012199119,"about_ca_system_score_gemma":0.0002965881,"threshold_uncertainty_score":0.022414327},"labels":[],"label_agreement":null},{"id":"W3083946060","doi":"10.3847/1538-4357/ababa1","title":"Multimessenger Gravitational-wave Searches with Pulsar Timing Arrays: Application to 3C 66B Using the NANOGrav 11-year Data Set","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"Office of Experimental Program to Stimulate Competitive Research; Office of Naval Research; Science and Technology Facilities Council; Flatiron Health; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; West Virginia University; Canadian Institute for Advanced Research; California Institute of Technology; National Aeronautics and Space Administration; Oak Ridge Associated Universities; University of Central Florida; National Science Foundation","keywords":"Physics; Pulsar; Astrophysics; Gravitational wave; Supermassive black hole; Astronomy; Binary pulsar; LIGO; Binary black hole; Millisecond pulsar; Galaxy; Gravitational-wave observatory","score_opus":0.09133709943566685,"score_gpt":0.3595514115901882,"score_spread":0.26821431215452135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3083946060","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99278635,0.00018566375,0.002529691,0.0001060903,0.000012217226,0.000027149053,0.002205209,0.00021772116,0.0019299432],"genre_scores_gemma":[0.97589046,0.00010642502,0.016307324,0.000037988284,0.000019416475,0.000025116413,0.0071083438,0.00005610312,0.0004487306],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959487,0.000110225454,0.000027857215,0.0001035814,0.000115277464,0.00004822765],"domain_scores_gemma":[0.99864954,0.00046808633,0.00025877389,0.00024241238,0.00017501853,0.00020621634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011035773,0.00033548172,0.00037197417,0.0023639402,0.0006330274,0.0009931665,0.0005276031,0.00040508056,0.00072391075],"category_scores_gemma":[0.0022936095,0.0002614711,0.0004012679,0.002242408,0.00027546787,0.00052062224,0.00115167,0.0003667451,0.00027272943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008486516,0.0003077682,0.8631529,0.00011970234,0.00037740695,0.00086624065,0.00041414384,0.043676022,0.017249634,0.0020607538,0.0034107051,0.06751602],"study_design_scores_gemma":[0.00021987096,0.0002347981,0.75578785,0.0000661369,0.00014045328,0.0005365876,0.00052656274,0.2198469,0.0101946145,0.0015755913,0.0107650915,0.000105629326],"about_ca_topic_score_codex":0.032677468,"about_ca_topic_score_gemma":0.061880253,"teacher_disagreement_score":0.032677468,"about_ca_system_score_codex":0.0005623153,"about_ca_system_score_gemma":0.00060094375,"threshold_uncertainty_score":0.06497455},"labels":[],"label_agreement":null},{"id":"W3084289624","doi":"10.3847/1538-4357/abb46f","title":"Measurement of Low-energy Cosmic-Ray Electron and Positron Spectra at 1 au with the AESOP-Lite Spectrometer","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Aeronautics and Space Administration","keywords":"Physics; Cosmic ray; Spectrometer; Cherenkov detector; Electron; Positron; Spectral line; Electron spectrometer; Rigidity (electromagnetism); Nuclear physics; Cherenkov radiation; Atomic physics; Detector; Astronomy; Optics; Cathode ray","score_opus":0.006815518771713547,"score_gpt":0.1848412504683692,"score_spread":0.17802573169665564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084289624","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98994863,0.00019317845,0.0032282083,0.000046308032,0.00001417367,0.000019333558,0.00090061076,0.00017815147,0.00547138],"genre_scores_gemma":[0.99276054,0.000080468824,0.0052414197,0.00001883627,0.000009605068,0.0000107898595,0.00061606424,0.000031665717,0.0012306718],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99987984,0.000014716837,0.0000036468227,0.000037185604,0.00004849288,0.000016046679],"domain_scores_gemma":[0.9997973,0.00004814513,0.000030213563,0.000034500827,0.000058433943,0.00003138135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018781354,0.00027677682,0.00025150622,0.0008257893,0.0003251837,0.00031431418,0.00026163372,0.00025683545,0.0015447395],"category_scores_gemma":[0.00032232184,0.0001699641,0.0001470775,0.0003746545,0.00016693253,0.00034682566,0.00034685095,0.0003219598,0.0002409852],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009656424,0.00018051564,0.13110459,0.000105861,0.00014097344,0.0005005904,0.00047982397,0.0019028051,0.8357725,0.0012892329,0.0009794147,0.026577951],"study_design_scores_gemma":[0.00006898864,0.0007814802,0.6410898,0.000023602257,0.00008625652,0.0009779371,0.0001806433,0.014919876,0.330302,0.0003639794,0.011156608,0.000048762973],"about_ca_topic_score_codex":0.0010809766,"about_ca_topic_score_gemma":0.002309695,"teacher_disagreement_score":0.0015447395,"about_ca_system_score_codex":0.00027749865,"about_ca_system_score_gemma":0.000094234005,"threshold_uncertainty_score":0.005167663},"labels":[],"label_agreement":null},{"id":"W3084343137","doi":"10.3847/1538-4357/abb6f7","title":"The Hidden Past of M92: Detection and Characterization of a Newly Formed 17° Long Stellar Stream Using the Canada–France Imaging Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; Dalhousie University; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Globular cluster; Photometry (optics); Stars; Proper motion; Velocity dispersion; Horizontal branch; Stellar mass; Open cluster","score_opus":0.010665366860852994,"score_gpt":0.20547796786661027,"score_spread":0.19481260100575729,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084343137","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985568,0.00006175476,0.00009073442,0.000023717708,0.0000010329487,0.000005015657,0.0003773994,0.00001177415,0.00087168824],"genre_scores_gemma":[0.99884903,0.000032379972,0.00026403792,0.000009325361,0.0000022819806,0.0000023156829,0.00055863126,0.0000033503557,0.0002786202],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990034,0.0000046678265,0.0000023087987,0.000020432255,0.000037899124,0.000034403245],"domain_scores_gemma":[0.99963665,0.00001724104,0.0000735599,0.000024887451,0.00011921053,0.00012848544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013314004,0.00015804332,0.00017862779,0.001216209,0.0006197046,0.00059892336,0.00027393602,0.00020058392,0.0008267593],"category_scores_gemma":[0.00036048074,0.0001016752,0.00012902422,0.0009881317,0.00029586203,0.0001778304,0.00048153865,0.00016605937,0.00025211365],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000904109,0.000020073374,0.9744374,0.000009942776,0.000016855009,0.0003760285,0.0003617383,0.000216446,0.017575998,0.00016535285,0.0004156116,0.0063141366],"study_design_scores_gemma":[0.0000020795032,0.000009902984,0.99806994,0.0000032311657,0.000004442637,0.00009321745,0.00013437362,0.00034126415,0.00046523483,0.000011519236,0.0008623162,0.0000025444829],"about_ca_topic_score_codex":0.31607157,"about_ca_topic_score_gemma":0.55055535,"teacher_disagreement_score":0.31607157,"about_ca_system_score_codex":0.0014865262,"about_ca_system_score_gemma":0.0008632331,"threshold_uncertainty_score":0.6284636},"labels":[],"label_agreement":null},{"id":"W3084522355","doi":"10.3847/1538-4357/abb80c","title":"SDSS-IV MaNGA: The Nature of an Off-galaxy H<sub>α</sub> Blob—A Multiwavelength View of Offset Cooling in a Merging Galaxy Group","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Active galactic nucleus; Galaxy group; Galaxy formation and evolution; Offset (computer science); Cooling flow; Ionization; Molecular cloud","score_opus":0.007229453961360433,"score_gpt":0.21496593528010963,"score_spread":0.2077364813187492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084522355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960173,0.0001884622,0.00018047824,0.00006413382,0.000003033267,0.0000052455957,0.00014368576,0.000025130043,0.0033725027],"genre_scores_gemma":[0.9994166,0.00003279131,0.00021778772,0.000016708662,0.0000074777945,0.000001779864,0.0000808431,0.0000036403949,0.0002223146],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997306,0.0000028632123,0.0000011379658,0.000007986355,0.0000037226914,0.000011176103],"domain_scores_gemma":[0.9998739,0.000015788044,0.0000408347,0.000008597247,0.000011148159,0.00004965629],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111952984,0.000093320894,0.000070282884,0.00083815394,0.0002589261,0.0003867685,0.00014964436,0.0001613086,0.0012622933],"category_scores_gemma":[0.00010903625,0.00010227781,0.00009166543,0.0002687087,0.00024214417,0.0002246887,0.00026095708,0.0001424529,0.00019992882],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041294508,0.000050548184,0.85061294,0.00006546307,0.000058544054,0.0030445163,0.0013812148,0.000515354,0.12922285,0.0012303257,0.0011806249,0.01222465],"study_design_scores_gemma":[0.0000029828489,0.000016583199,0.99680436,0.000006772633,0.0000072042617,0.0004734711,0.0003010854,0.00062107464,0.0007881878,0.000110021676,0.0008655249,0.0000026902164],"about_ca_topic_score_codex":0.0051962654,"about_ca_topic_score_gemma":0.006169211,"teacher_disagreement_score":0.0051962654,"about_ca_system_score_codex":0.00029569227,"about_ca_system_score_gemma":0.00007002438,"threshold_uncertainty_score":0.010332048},"labels":[],"label_agreement":null},{"id":"W3084642752","doi":"10.3847/1538-4357/abb67d","title":"Super Star Clusters in the Central Starburst of NGC 4945","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Galaxy; Submillimeter Array; Millimeter; Stars; Star formation; Star cluster; Stellar mass; Astronomy; Full width at half maximum","score_opus":0.009594711176415293,"score_gpt":0.20264252740485786,"score_spread":0.19304781622844255,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084642752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996013,0.000028917451,0.000044756114,0.0000072826315,0.0000010061111,0.0000012540879,0.000044900185,0.00000768392,0.00026296778],"genre_scores_gemma":[0.99974424,0.000012236282,0.00006816433,0.0000046167993,0.000002489819,8.599719e-7,0.00009924787,0.0000010817596,0.000066932604],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999176,0.000007579102,0.0000050020763,0.000025076515,0.0000248752,0.000019834282],"domain_scores_gemma":[0.9995889,0.000039796476,0.00017780485,0.00002785232,0.00003396874,0.00013165723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000094798204,0.00013271262,0.00015116455,0.0005956724,0.00033933832,0.0004966342,0.00018852473,0.00015892462,0.0013967155],"category_scores_gemma":[0.00027310516,0.00012439997,0.00011596411,0.0004023899,0.00017435006,0.00014810839,0.00039913756,0.000093858784,0.00019378956],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016212335,0.00003967033,0.96573615,0.000012257902,0.000043973658,0.0006263557,0.0004236452,0.00035789885,0.026773652,0.00021551391,0.00038146818,0.005227323],"study_design_scores_gemma":[0.0000029805767,0.00002216848,0.9986951,0.0000019779627,0.000006470842,0.00018277628,0.000090550224,0.00036872862,0.0003682812,0.000036380043,0.00022285923,0.000001637529],"about_ca_topic_score_codex":0.009323247,"about_ca_topic_score_gemma":0.012923872,"teacher_disagreement_score":0.009323247,"about_ca_system_score_codex":0.00025263627,"about_ca_system_score_gemma":0.00009133447,"threshold_uncertainty_score":0.018537939},"labels":[],"label_agreement":null},{"id":"W3084647316","doi":"10.3847/1538-4357/abb611","title":"Swift/BAT and RXTE/ASM Observations of the 35 day X-Ray Cycle of Hercules X-1","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Orbital period; Gaussian; Accretion (finance); Noise (video); Phase (matter); Accretion disc; Binary number","score_opus":0.02111485482525407,"score_gpt":0.22074984480501755,"score_spread":0.19963498997976348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084647316","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974987,0.000081622034,0.00032802366,0.000031481395,0.000006972789,0.0000071173567,0.0010313904,0.00007431792,0.0009403939],"genre_scores_gemma":[0.99588025,0.000031104282,0.00060835894,0.000015948279,0.000016389193,0.000010185573,0.0029726115,0.000035037443,0.00043007926],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998623,0.000017200979,0.000009883796,0.000043190954,0.000036926518,0.000030450567],"domain_scores_gemma":[0.9992636,0.000080259386,0.00031078805,0.00006632374,0.00013372871,0.00014520544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037592568,0.00023948516,0.00018459825,0.0015889351,0.00021779595,0.0004622787,0.00019558347,0.00024985397,0.0009802735],"category_scores_gemma":[0.0008202716,0.00015754589,0.00030139202,0.0008531965,0.00015138886,0.00021774136,0.00035322737,0.00021049716,0.00023011805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019266263,0.000069428366,0.9600333,0.000036981593,0.00009864232,0.0002525496,0.00024366085,0.0047083013,0.01597001,0.00054530095,0.0027017123,0.015147366],"study_design_scores_gemma":[0.0000030538338,0.000013031672,0.9961804,0.000002480617,0.000005023755,0.000057215966,0.000012830884,0.002768899,0.00036754523,0.000033279382,0.0005529133,0.0000033497927],"about_ca_topic_score_codex":0.0063676992,"about_ca_topic_score_gemma":0.0077962563,"teacher_disagreement_score":0.0063676992,"about_ca_system_score_codex":0.00036110726,"about_ca_system_score_gemma":0.00018958685,"threshold_uncertainty_score":0.012661278},"labels":[],"label_agreement":null},{"id":"W3084763888","doi":"10.3847/1538-4357/abb8d5","title":"Progenitors of Type IIb Supernovae. II. Observable Properties","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Quest High Performance Computing; Purdue University; Fonds Wetenschappelijk Onderzoek; Canadian Institute for Advanced Research; Northwestern University; National Science Foundation","keywords":"Supernova; Metallicity; Observable; Stars; Binary number; Population; Progenitor; Stellar evolution","score_opus":0.03281846276174336,"score_gpt":0.2243954060630529,"score_spread":0.19157694330130953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084763888","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99424356,0.00021459053,0.0028432056,0.00002479895,0.0000014341688,0.000015309724,0.000573183,0.000035356505,0.0020485364],"genre_scores_gemma":[0.99875104,0.000063191925,0.0004754218,0.0000034344093,0.0000020881107,0.000005963481,0.0005027996,0.000007265668,0.00018868198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979347,0.000037836282,0.000015077327,0.000076790486,0.000036099085,0.000040722065],"domain_scores_gemma":[0.9987036,0.00035938583,0.00048113387,0.00019572431,0.00011043585,0.0001496416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000654135,0.00045630176,0.00040595868,0.0008099446,0.0003209775,0.0015299136,0.0009950437,0.00037798655,0.0030494859],"category_scores_gemma":[0.0022600484,0.00034745177,0.00053974916,0.0005451968,0.00045816545,0.00065564323,0.001030357,0.00033707908,0.0004818157],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022498005,0.0000596842,0.9121706,0.00007333984,0.00009287555,0.00024639125,0.00013067458,0.05949786,0.008923496,0.0061204378,0.00022221057,0.01223745],"study_design_scores_gemma":[0.00006543909,0.0002525227,0.72820836,0.00006304473,0.00013302236,0.0015134922,0.0005471814,0.24237576,0.0061728396,0.018349357,0.0022766255,0.0000423448],"about_ca_topic_score_codex":0.0018791273,"about_ca_topic_score_gemma":0.0014279914,"teacher_disagreement_score":0.0030494859,"about_ca_system_score_codex":0.00042804703,"about_ca_system_score_gemma":0.00022555972,"threshold_uncertainty_score":0.010201573},"labels":[],"label_agreement":null},{"id":"W3084996964","doi":"10.3847/1538-4357/ac0aeb","title":"The Nickel Mass Distribution of Stripped-envelope Supernovae: Implications for Additional Power Sources","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Gordon and Betty Moore Foundation","keywords":"Physics; Dimensionless quantity; Supernova; Luminosity; Astrophysics; Envelope (radar); Nickel; Analytical Chemistry (journal); Atomic physics; Thermodynamics; Materials science","score_opus":0.014177112939453295,"score_gpt":0.24944771830136056,"score_spread":0.23527060536190728,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3084996964","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99379504,0.00017775745,0.0046526818,0.000023387502,0.0000023880493,0.0000061929704,0.00017034894,0.000054115175,0.0011180736],"genre_scores_gemma":[0.9988311,0.00005620884,0.00076384225,0.000006282571,0.0000034197153,0.000004073246,0.00015474991,0.000012887889,0.00016735982],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984384,0.000022395241,0.000012757784,0.00006170523,0.00004160201,0.000017743298],"domain_scores_gemma":[0.99882,0.0003096492,0.00034870883,0.000306305,0.00013473419,0.00008046826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074717234,0.00037954192,0.0003128096,0.0008634852,0.00028959816,0.0007451639,0.00076754106,0.00022643911,0.001132494],"category_scores_gemma":[0.0020504722,0.00022925215,0.0004822373,0.0004995558,0.00046869516,0.0006454425,0.00060842,0.00024256516,0.00029077564],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027402877,0.00003877528,0.94549316,0.00006284889,0.000115005874,0.00030381954,0.00017562059,0.010013944,0.02871143,0.0021991662,0.00009421608,0.012518093],"study_design_scores_gemma":[0.000027679911,0.00018548312,0.87119365,0.000036432193,0.00009599849,0.00046186583,0.00024069086,0.08059246,0.040249653,0.0049188905,0.0019589397,0.000038232713],"about_ca_topic_score_codex":0.0012026357,"about_ca_topic_score_gemma":0.00088327477,"teacher_disagreement_score":0.0012026357,"about_ca_system_score_codex":0.0003876638,"about_ca_system_score_gemma":0.00014839704,"threshold_uncertainty_score":0.00395149},"labels":[],"label_agreement":null},{"id":"W3085029108","doi":"10.3847/1538-4357/abb673","title":"The Massive and Distant Clusters of WISE Survey. X. Initial Results from a Sunyaev–Zeldovich Effect Study of Massive Galaxy Clusters at z &gt; 1 Using MUSTANG2 on the GBT","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Redshift; Galaxy cluster; Galaxy; Cluster (spacecraft); South Pole Telescope; Sigma; Redshift survey; Telescope; Astronomy","score_opus":0.018425266928618296,"score_gpt":0.24288858738952462,"score_spread":0.22446332046090633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3085029108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99910307,0.000027864015,0.00007014091,0.000015595499,0.0000012817068,0.000003764233,0.00041457993,0.000006234723,0.0003574845],"genre_scores_gemma":[0.9981142,0.000024634286,0.0002035108,0.000007872044,0.000004138918,0.000004313845,0.0012153861,0.0000048918178,0.00042098865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982315,0.000029752895,0.0000070470514,0.000046481986,0.000040546332,0.00005306552],"domain_scores_gemma":[0.9993863,0.00005275996,0.00014647901,0.00006567216,0.000049040562,0.00029961104],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031662403,0.00025188035,0.00024817212,0.0008523822,0.0005575452,0.00038366063,0.00022277546,0.00012767393,0.0008557319],"category_scores_gemma":[0.00047903392,0.0001736663,0.00019048032,0.0006404848,0.00029362997,0.00025999278,0.00079161907,0.00021047467,0.00018977278],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028665044,0.000030964096,0.9891009,0.0000095908845,0.000033339595,0.00014137034,0.00044618605,0.00018907162,0.0056208847,0.00023140346,0.00045993354,0.0034496875],"study_design_scores_gemma":[0.0000024101562,0.00001389674,0.9991047,5.539142e-7,0.000004332365,0.000028868182,0.000054072483,0.00010605502,0.00034235258,0.0000114524455,0.00033003214,0.0000012912897],"about_ca_topic_score_codex":0.018741835,"about_ca_topic_score_gemma":0.04540672,"teacher_disagreement_score":0.018741835,"about_ca_system_score_codex":0.0003553632,"about_ca_system_score_gemma":0.00019773818,"threshold_uncertainty_score":0.03726554},"labels":[],"label_agreement":null},{"id":"W3085611766","doi":"10.3847/1538-4357/abba1a","title":"Galaxy and Mass Assembly (GAMA): A WISE Study of the Activity of Emission-line Systems in G23","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"University of California, Los Angeles; Jet Propulsion Laboratory; National Research Foundation; Australian Government; National Aeronautics and Space Administration; California Institute of Technology; Science and Technology Facilities Council; Johns Hopkins University","keywords":"Galaxy; Active galactic nucleus; Luminosity; Photometry (optics); Spurious relationship; Luminous infrared galaxy; Galaxy formation and evolution; Extragalactic astronomy","score_opus":0.013822768557742423,"score_gpt":0.23220295766382995,"score_spread":0.21838018910608753,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3085611766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987166,0.00007984574,0.000090022804,0.000014340777,4.8772375e-7,0.0000054862912,0.0006371694,0.000010332704,0.00044568814],"genre_scores_gemma":[0.9983557,0.000034658064,0.00032079234,0.000009737579,0.0000023735724,0.000008193298,0.0010743707,0.000008935244,0.00018523503],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966276,0.000067569505,0.000014448002,0.00009206048,0.00007281313,0.000090439025],"domain_scores_gemma":[0.99915683,0.00009333578,0.00028173035,0.00011283662,0.00010201992,0.00025317346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028282573,0.00033082382,0.00034597068,0.0035077713,0.0005146774,0.00069299096,0.0003333951,0.00024698785,0.001678241],"category_scores_gemma":[0.0012216909,0.00013211642,0.00033327052,0.0025261971,0.00029688972,0.00037942143,0.00096673076,0.00025542933,0.000709963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056366265,0.000020234153,0.9880427,0.00001314323,0.000059392016,0.00016244425,0.00042911796,0.000106685846,0.0049386653,0.00017927124,0.0002604819,0.0057313945],"study_design_scores_gemma":[7.3367363e-7,0.000020112167,0.99899215,0.0000013833408,0.000005082495,0.00013536045,0.00016479848,0.000111785055,0.00017314698,0.000024516094,0.00036890493,0.0000019970837],"about_ca_topic_score_codex":0.012296558,"about_ca_topic_score_gemma":0.016425058,"teacher_disagreement_score":0.012296558,"about_ca_system_score_codex":0.00037296145,"about_ca_system_score_gemma":0.000188567,"threshold_uncertainty_score":0.024449944},"labels":[],"label_agreement":null},{"id":"W3085944779","doi":"10.3847/1538-4357/abd32b","title":"X-Ray Spectroscopy of the Highly Magnetized Pulsar PSR J1846-0258, Its Wind Nebula, and Hosting Supernova Remnant Kes 75","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"National Aeronautics and Space Administration","keywords":"Physics; Pulsar; Magnetar; Pulsar wind nebula; Astrophysics; Supernova remnant; Neutron star; Nebula; Astronomy; Flux (metallurgy); Supernova; Stars","score_opus":0.01097517715942026,"score_gpt":0.22551790031900157,"score_spread":0.2145427231595813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3085944779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993298,0.00004652396,0.00006155975,0.0000050208946,0.0000015598376,0.0000019808476,0.00008175284,0.000009176186,0.0004626557],"genre_scores_gemma":[0.99868685,0.000051275394,0.00028966795,0.00001453386,0.0000059505423,0.0000029286034,0.00042986497,0.0000049375312,0.00051396684],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999455,0.0000035596745,0.0000047128037,0.000013880185,0.000019346484,0.00001300928],"domain_scores_gemma":[0.99989665,0.000009037642,0.00003470848,0.0000104586115,0.00001386067,0.000035373334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013798015,0.00023704804,0.00023064193,0.00068738294,0.00025482147,0.00032512788,0.00024413201,0.0001985127,0.0011219531],"category_scores_gemma":[0.00017876085,0.00015428568,0.00011344037,0.00034296227,0.00013291501,0.00016110647,0.00034473898,0.00016460774,0.00027600024],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046970655,0.00035579043,0.48455948,0.00007800703,0.0001320462,0.0045101093,0.00034493566,0.0008002247,0.49344897,0.00028846852,0.00066772196,0.014344622],"study_design_scores_gemma":[0.000015772825,0.000197873,0.98846126,0.000005062409,0.00001898073,0.0013220046,0.00011610553,0.0006189553,0.0077954927,0.000033459157,0.0014101255,0.000004912489],"about_ca_topic_score_codex":0.0010021634,"about_ca_topic_score_gemma":0.0019424768,"teacher_disagreement_score":0.0011219531,"about_ca_system_score_codex":0.00013591225,"about_ca_system_score_gemma":0.00006775183,"threshold_uncertainty_score":0.003753364},"labels":[],"label_agreement":null},{"id":"W3086268987","doi":"10.3847/1538-4357/abb6fe","title":"Young Faithful: The Eruptions of EC 53 as It Cycles through Filling and Draining the Inner Disk","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Accretion (finance); Accretion disc; Young stellar object; Schematic; Luminosity; Stellar mass","score_opus":0.02335404919617962,"score_gpt":0.2662197018982188,"score_spread":0.2428656527020392,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3086268987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967608,0.000104987026,0.0008110905,0.00001885109,0.0000035181763,0.0000052267874,0.00019800354,0.00005173311,0.002045766],"genre_scores_gemma":[0.9993394,0.00002696334,0.00031154137,0.000007652468,0.0000027708638,0.0000015339715,0.00010109985,0.0000054004395,0.00020359279],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996305,0.0000035222163,0.0000020939892,0.00001489056,0.000007619423,0.000008728425],"domain_scores_gemma":[0.99976045,0.00003986268,0.000105495266,0.000033219912,0.000028234892,0.000032718646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012009009,0.00012673184,0.00011510447,0.0003141749,0.00017794219,0.0004344257,0.00016598165,0.00023289368,0.0010106749],"category_scores_gemma":[0.000488571,0.00006843749,0.00009687696,0.00024650205,0.00017717575,0.00020297631,0.00018829192,0.00017568795,0.00022187435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020005475,0.00003959919,0.8509856,0.00005663624,0.000050822608,0.0010075221,0.00050593994,0.0022045705,0.10960346,0.001020017,0.00073943817,0.033586457],"study_design_scores_gemma":[0.0000016516834,0.00003313909,0.9912471,0.00000808933,0.000010863916,0.0003258261,0.00012815093,0.0027013815,0.0041577267,0.00017006492,0.0012110003,0.0000050082335],"about_ca_topic_score_codex":0.0021070894,"about_ca_topic_score_gemma":0.0026998355,"teacher_disagreement_score":0.0021070894,"about_ca_system_score_codex":0.00023312873,"about_ca_system_score_gemma":0.000052256753,"threshold_uncertainty_score":0.0041896105},"labels":[],"label_agreement":null},{"id":"W3086857322","doi":"10.3847/1538-4357/abb77b","title":"An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio Correlation for High-redshift Dusty Star-forming Galaxies","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"Science and Technology Facilities Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Jansky; Galaxy; Redshift; Cosmology; Luminous infrared galaxy; Radio galaxy; Population; Interstellar medium; COSMIC cancer database","score_opus":0.018233842663965095,"score_gpt":0.23839426901310068,"score_spread":0.22016042634913557,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3086857322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971167,0.00012016972,0.00024543444,0.000026690517,0.000003472133,0.0000050875806,0.0012756756,0.000024283088,0.0011824834],"genre_scores_gemma":[0.99774975,0.000029357767,0.00021517176,0.000017312314,0.000010501531,0.000004383283,0.0016630713,0.0000057109987,0.00030487723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996779,0.00006586082,0.000016896982,0.00008831662,0.0000794415,0.00007154513],"domain_scores_gemma":[0.99814594,0.00023140883,0.00068982947,0.0002659796,0.00034516433,0.00032170277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043117604,0.00019544702,0.00019573572,0.0022144427,0.0002759834,0.00051220733,0.00029201107,0.00016156367,0.0018594259],"category_scores_gemma":[0.001074962,0.000116081384,0.0001814719,0.0013464687,0.00022950934,0.00024386263,0.00043705976,0.00016274494,0.0005689185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000021725533,0.000008788185,0.99625254,0.0000052200235,0.000021431506,0.00002399025,0.00003369036,0.00011585022,0.0011556464,0.000057975598,0.0004056782,0.0018973416],"study_design_scores_gemma":[0.0000011923262,0.000003986907,0.9993692,0.0000018015836,0.0000044211997,0.000020213614,0.000024779394,0.0002582417,0.0000997263,0.000011471832,0.00020380011,0.0000011534104],"about_ca_topic_score_codex":0.01702072,"about_ca_topic_score_gemma":0.030305916,"teacher_disagreement_score":0.01702072,"about_ca_system_score_codex":0.00022679326,"about_ca_system_score_gemma":0.00017151593,"threshold_uncertainty_score":0.03384334},"labels":[],"label_agreement":null},{"id":"W3086947203","doi":"10.3847/1538-4357/abab96","title":"The Blue Compact Dwarf Galaxy VCC 848 Formed by Dwarf–Dwarf Merging: H i Gas, Star Formation, and Numerical Simulations","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Dwarf galaxy; Dwarf spheroidal galaxy; Surface brightness; Astronomy; Luminosity; Galaxy; Star formation; Interacting galaxy","score_opus":0.010695881711943082,"score_gpt":0.22667908155619368,"score_spread":0.2159831998442506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3086947203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930837,0.000099086035,0.0011554415,0.00012590777,0.000014056498,0.000020044074,0.0003605889,0.000110600675,0.005030574],"genre_scores_gemma":[0.9975611,0.000044250246,0.001498512,0.000038091166,0.000011328748,0.000018033568,0.00026669368,0.000025595331,0.000536405],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999897,0.000022437456,0.000004619831,0.000017953525,0.000018447927,0.00003945501],"domain_scores_gemma":[0.9992156,0.00041698886,0.000098186814,0.000048109505,0.000085952954,0.0001351134],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030749288,0.00041459978,0.0005591649,0.0007142945,0.0007219672,0.000737052,0.0013058486,0.0008583737,0.0019849222],"category_scores_gemma":[0.001179701,0.00028926233,0.0005289438,0.00054681697,0.00071988994,0.0003545996,0.0006874147,0.00064430793,0.00017870682],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014835343,0.000162683,0.02670888,0.00004459202,0.00007370613,0.0002728752,0.0000949136,0.9660203,0.002000498,0.0021424715,0.00047841514,0.0018522856],"study_design_scores_gemma":[0.000037900558,0.00003361392,0.003983422,0.0000044614544,0.000012034398,0.000018972712,0.00004835924,0.994894,0.0002853031,0.00045992283,0.00021388663,0.000008062456],"about_ca_topic_score_codex":0.053250846,"about_ca_topic_score_gemma":0.023819573,"teacher_disagreement_score":0.053250846,"about_ca_system_score_codex":0.0013821773,"about_ca_system_score_gemma":0.00071897364,"threshold_uncertainty_score":0.10588181},"labels":[],"label_agreement":null},{"id":"W3086951273","doi":"10.3847/1538-4357/abb80b","title":"Subaru High-z Exploration of Low-luminosity Quasars (SHELLQs). XI. Proximity Zone Analysis for Faint Quasar Spectra at z ∼ 6","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; National Central University; Eötvös Loránd Tudományegyetem; Academia Sinica; Space Telescope Science Institute; Ministry of Education, Culture, Sports, Science and Technology; Princeton University; Johns Hopkins University; Japan Society for the Promotion of Science; Queen's University Belfast; National Aeronautics and Space Administration; Queen's University; Cabinet Office, Government of Japan; Durham University; Smithsonian Institution; Toray Science Foundation; National Science Foundation","keywords":"Physics; Quasar; Astrophysics; Spectral line; Luminosity; OVV quasar; Astronomy; Galaxy","score_opus":0.017350669640726957,"score_gpt":0.2218447014307302,"score_spread":0.20449403179000325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3086951273","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99659735,0.00020904928,0.0011673005,0.000022571036,0.000002409226,0.000009382324,0.0009273149,0.000057914804,0.0010067348],"genre_scores_gemma":[0.99741626,0.000042381813,0.001294645,0.000009647426,0.0000055148957,0.0000058087703,0.0008622274,0.000008820092,0.00035463445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998092,0.000042404157,0.000012596648,0.000049779388,0.00004554976,0.000040460054],"domain_scores_gemma":[0.99887747,0.00021016235,0.0004280436,0.00011333927,0.00011272462,0.0002581592],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062114885,0.000231701,0.00018941755,0.002303001,0.00025357524,0.0004977133,0.00027752962,0.00015779711,0.0015883038],"category_scores_gemma":[0.00081061135,0.00010177841,0.00030380758,0.0007284692,0.00017865315,0.00033211062,0.0010186101,0.00023020801,0.00036282573],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001170396,0.000023315635,0.972451,0.000027241354,0.00003732913,0.00013403628,0.00015240462,0.00014459383,0.0084061865,0.00011535106,0.00018432169,0.01820711],"study_design_scores_gemma":[0.0000012998521,0.00002119578,0.9986533,0.0000017089053,0.000008249282,0.00010015468,0.000040503328,0.00022005083,0.0006810515,0.000034570898,0.00023634115,0.0000015773351],"about_ca_topic_score_codex":0.0021393695,"about_ca_topic_score_gemma":0.0036640079,"teacher_disagreement_score":0.002303001,"about_ca_system_score_codex":0.00011392819,"about_ca_system_score_gemma":0.00009205734,"threshold_uncertainty_score":0.005313456},"labels":[],"label_agreement":null},{"id":"W3087050878","doi":"10.3847/1538-4357/abba76","title":"ALMA Observations of the Inner Cavity in the Protoplanetary Disk around Sz 84","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Protoplanetary disk; T Tauri star; Cosmic dust; Spectral energy distribution; Circumstellar dust; RADIUS; Infrared; Grain growth; Photoevaporation; Grain size","score_opus":0.02145116926642968,"score_gpt":0.24126337658239802,"score_spread":0.21981220731596834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087050878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99900144,0.000029125458,0.000078044104,0.000014188389,0.00000221278,0.0000033417748,0.0001196387,0.0000235539,0.00072835013],"genre_scores_gemma":[0.9992873,0.000022119666,0.00027567268,0.000010709887,0.00000685483,0.0000046357472,0.0001852352,0.0000033622532,0.0002041092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999548,0.000003210507,0.0000018006358,0.0000110147375,0.000014433848,0.00001473114],"domain_scores_gemma":[0.99981433,0.000018947507,0.000049377373,0.000019216634,0.000036614307,0.000061601815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009975932,0.00015888327,0.00024217441,0.0005890631,0.00046957168,0.00028589304,0.0003234624,0.00023249301,0.00071146426],"category_scores_gemma":[0.00024230978,0.00014007108,0.00015824448,0.0003276127,0.00017070668,0.0001800443,0.0005045978,0.00022304538,0.0002496211],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010603591,0.00022883787,0.5911051,0.00009699721,0.00013305889,0.0017220118,0.0013741669,0.0016370465,0.3746735,0.000416582,0.0014729162,0.026079532],"study_design_scores_gemma":[0.000025091049,0.00010698752,0.99523455,0.0000050509593,0.00002246114,0.00013689317,0.0001827462,0.001279101,0.0021665161,0.00006552302,0.00076945696,0.0000055783275],"about_ca_topic_score_codex":0.0045837397,"about_ca_topic_score_gemma":0.0071749757,"teacher_disagreement_score":0.0045837397,"about_ca_system_score_codex":0.00031835446,"about_ca_system_score_gemma":0.00014428516,"threshold_uncertainty_score":0.009114146},"labels":[],"label_agreement":null},{"id":"W3087070468","doi":"10.3847/1538-4357/abb94f","title":"The Discovery of Nulling and Mode-switching Pulsars with CHIME/Pulsar","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McGill University; Herzberg Institute of Astrophysics; University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Pulsar; Sky; Millisecond pulsar; Population; X-ray pulsar; Mode (computer interface)","score_opus":0.010332321688578805,"score_gpt":0.28514967901597876,"score_spread":0.2748173573274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087070468","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996977,0.00012845559,0.0011232464,0.000051407602,0.000019151248,0.000013142139,0.00024889302,0.00006852448,0.0013701557],"genre_scores_gemma":[0.99818665,0.000035480884,0.00093642215,0.00004835498,0.000012808261,0.0000064874016,0.00038484763,0.000014554939,0.00037435812],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975044,0.000015129885,0.000011648999,0.00006796761,0.000085815605,0.000068917965],"domain_scores_gemma":[0.9992428,0.000116366056,0.0001906096,0.00014357237,0.00015044792,0.00015622326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040575286,0.00020170028,0.00033190424,0.0011767144,0.000706646,0.0007822549,0.00030860127,0.00034760652,0.0008725775],"category_scores_gemma":[0.0010904454,0.00018808074,0.00014294042,0.0007515703,0.00078031875,0.00022153612,0.0007359094,0.0004560978,0.00022635687],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006101231,0.00013267391,0.58086234,0.00004774462,0.00012576705,0.0013566363,0.00088360877,0.00017317262,0.37800306,0.000756374,0.0010749944,0.035973433],"study_design_scores_gemma":[0.000012574231,0.000092927476,0.9803986,0.0000046548666,0.000022874026,0.0011411252,0.000146167,0.00041680541,0.01554799,0.00019937301,0.0020015028,0.000015338263],"about_ca_topic_score_codex":0.004117532,"about_ca_topic_score_gemma":0.0052057565,"teacher_disagreement_score":0.004117532,"about_ca_system_score_codex":0.00025317978,"about_ca_system_score_gemma":0.00019819687,"threshold_uncertainty_score":0.008187115},"labels":[],"label_agreement":null},{"id":"W3087196908","doi":"10.3847/1538-4357/abb6fc","title":"The MAVERIC Survey: New Compact Binaries Revealed by Deep Radio Continuum Observations of the Galactic Globular Cluster Terzan 5","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Globular cluster; Millisecond pulsar; Pulsar; Jansky; Star cluster; Population; Galaxy; Binary number","score_opus":0.02122408037956266,"score_gpt":0.2220029584256106,"score_spread":0.20077887804604794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087196908","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99889284,0.00018509553,0.00008896111,0.000013638687,0.0000033139386,0.0000048688476,0.00014323152,0.0000074369673,0.0006606186],"genre_scores_gemma":[0.99884665,0.00009261389,0.00019466107,0.000021773234,0.0000067145543,0.0000035210228,0.00056706514,0.0000033980523,0.0002636463],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986327,0.000012861982,0.000008692508,0.000044364842,0.000034442677,0.00003639527],"domain_scores_gemma":[0.99973303,0.000013330469,0.00010228768,0.000029070587,0.000025776786,0.00009653733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021509684,0.0002123056,0.00020016189,0.0012512435,0.00028292928,0.00057887,0.00028893875,0.00015607625,0.00072361727],"category_scores_gemma":[0.00027796708,0.00011399937,0.00013934639,0.00065237744,0.00018558338,0.00023386498,0.0007475245,0.00018556126,0.00018655491],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011399272,0.000037437723,0.97714376,0.000014757557,0.0000853045,0.00041147714,0.00038531696,0.000104572784,0.012117012,0.00014436853,0.00041415208,0.009027987],"study_design_scores_gemma":[0.0000041158896,0.000025344847,0.99829084,0.000003287086,0.000009073998,0.000269049,0.00014106228,0.000079105914,0.00014241917,0.000017026992,0.0010169666,0.0000016351405],"about_ca_topic_score_codex":0.003714648,"about_ca_topic_score_gemma":0.009672007,"teacher_disagreement_score":0.003714648,"about_ca_system_score_codex":0.00023941186,"about_ca_system_score_gemma":0.000112645066,"threshold_uncertainty_score":0.0073860288},"labels":[],"label_agreement":null},{"id":"W3087493313","doi":"10.3847/1538-4357/abb819","title":"The Massive Ancient Galaxies at z &gt; 3 NEar-infrared (MAGAZ3NE) Survey: Confirmation of Extremely Rapid Star Formation and Quenching Timescales for Massive Galaxies in the Early Universe*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Star formation; Galaxy; Redshift; Stars; Galaxy formation and evolution; Stellar evolution; Stellar mass; Spectral line","score_opus":0.016265774162878187,"score_gpt":0.21067341909590165,"score_spread":0.19440764493302345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087493313","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993974,0.000038310496,0.000074699004,0.000009862341,7.641794e-7,0.0000026623943,0.00021065853,0.00000697674,0.00025873465],"genre_scores_gemma":[0.99947864,0.000016944714,0.00017408852,0.000012198861,0.000002370335,0.0000020695022,0.00023987424,0.000001926194,0.00007201005],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976414,0.000034208137,0.000016498723,0.000049545077,0.000072905634,0.00006275509],"domain_scores_gemma":[0.9987185,0.00012158452,0.00047673637,0.00017384517,0.00016373317,0.0003456556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054132316,0.00016251481,0.00021809564,0.0010926551,0.00035471944,0.00038692317,0.0003037902,0.00024456883,0.0006234676],"category_scores_gemma":[0.0007077418,0.000101840546,0.00019823258,0.000656279,0.00031817786,0.0002234268,0.0005356603,0.0002618256,0.00021095284],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000080915386,0.000023052087,0.9894014,0.0000060964626,0.000016008486,0.000070214606,0.00016487324,0.000038320268,0.007441259,0.00005299758,0.00007832467,0.0026265737],"study_design_scores_gemma":[0.0000015107225,0.00001127294,0.9994425,7.193222e-7,0.0000025574936,0.00006278584,0.000027877417,0.00004733081,0.00029473653,0.00000710707,0.000100797675,7.1068763e-7],"about_ca_topic_score_codex":0.006672246,"about_ca_topic_score_gemma":0.0140350005,"teacher_disagreement_score":0.006672246,"about_ca_system_score_codex":0.00028676877,"about_ca_system_score_gemma":0.000119645454,"threshold_uncertainty_score":0.013266802},"labels":[],"label_agreement":null},{"id":"W3087789644","doi":"10.3847/1538-4357/abac0d","title":"Monitoring the Morphology of M87* in 2009–2017 with the Event Horizon Telescope","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Government of Canada; National Institutes of Natural Sciences; Consejo Nacional de Ciencia y Tecnología; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Japan Society for the Promotion of Science; Science and Technology Facilities Council; National Nuclear Security Administration; Institut Périmètre de physique théorique; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Universidad Nacional Autónoma de México; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Ministerio de Economía y Competitividad; European Southern Observatory; Korea Astronomy and Space Science Institute; Generalitat Valenciana; Chinese Academy of Sciences; Instituto de Astrofísica de Andalucía; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Harvard University; Toray Science Foundation; National Research Foundation; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; National Science Foundation; Compute Canada; National Astronomical Observatory of Japan; Associated Universities; University of Chicago; Vetenskapsrådet; U.S. Department of Energy; Kavli Foundation; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; Istituto Nazionale di Fisica Nucleare; Department of Science and Technology, Ministry of Science and Technology, India; Russian Science Foundation; Ministerio de Ciencia, Innovación y Universidades; Gordon and Betty Moore Foundation; Academia Sinica","keywords":"Position angle; Supermassive black hole; Brightness; Azimuth; Event horizon; Event (particle physics); Telescope; Position (finance)","score_opus":0.01872202764842446,"score_gpt":0.24288721101093402,"score_spread":0.22416518336250957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3087789644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970431,0.000047178608,0.0006359959,0.000056151843,0.000006073034,0.0000075187245,0.001070472,0.000063144354,0.0010704169],"genre_scores_gemma":[0.99709225,0.000027047312,0.00075950136,0.000019805455,0.0000121305,0.000005039505,0.0019557455,0.000015771519,0.000112648035],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974066,0.000028811806,0.000012742169,0.00005222077,0.00010090133,0.00006459046],"domain_scores_gemma":[0.9993,0.00006302216,0.0002162625,0.000107567255,0.00018857463,0.00012459375],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006270112,0.00017865332,0.00025310376,0.00077575207,0.000292463,0.00039894812,0.0004076378,0.00021004025,0.00038005298],"category_scores_gemma":[0.0008245139,0.00013383233,0.0002706969,0.0006245289,0.0003154781,0.0003043172,0.0005850058,0.00026682616,0.00023536415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029841423,0.00015899238,0.9365509,0.00004194058,0.00014872078,0.00049278844,0.0004888323,0.0048858933,0.035351917,0.00081133033,0.0033009308,0.017469365],"study_design_scores_gemma":[0.000009642313,0.000042367912,0.99043614,0.0000055036417,0.000019313198,0.000108399494,0.000099826495,0.005457691,0.0023794651,0.00010920374,0.0013250136,0.0000076087563],"about_ca_topic_score_codex":0.009726105,"about_ca_topic_score_gemma":0.020399613,"teacher_disagreement_score":0.009726105,"about_ca_system_score_codex":0.00062847935,"about_ca_system_score_gemma":0.00029245156,"threshold_uncertainty_score":0.019338965},"labels":[],"label_agreement":null},{"id":"W3088042883","doi":"10.3847/1538-4357/abb66e","title":"Erratum: “Far-infrared to Millimeter Data of Protoplanetary Disks: Dust Growth in the Taurus, Ophiuchus, and Chamaeleon I Star-forming Regions” (2017, ApJ, 849, 63)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Ophiuchus; Physics; Millimeter; Astrophysics; Astronomy; Far infrared; Star formation; Stars","score_opus":0.03187764410930487,"score_gpt":0.25958886288291,"score_spread":0.22771121877360512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3088042883","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.001063184,0.0011329268,0.00030084714,0.04238743,0.9213113,0.000025685145,0.011026887,0.00042852058,0.022323104],"genre_scores_gemma":[0.016414437,0.0059804595,0.00311899,0.07245351,0.15111929,0.0001283865,0.04003371,0.0022323977,0.70851886],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9983448,0.00012760087,0.00033927968,0.0002197084,0.0008118412,0.00015673754],"domain_scores_gemma":[0.9893468,0.0012685562,0.0006408848,0.000671834,0.0072658337,0.0008060782],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016141621,0.0017275861,0.0010575342,0.0037511862,0.0035167583,0.003913792,0.0018736362,0.0027772342,0.07655325],"category_scores_gemma":[0.014755874,0.00064422534,0.0008660636,0.0026284456,0.0009272537,0.0025063965,0.0018104049,0.004209719,0.06470864],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003669404,0.000009934199,0.00025434032,0.00004966029,0.0000035254357,0.0001106706,0.000014144222,0.0000334837,0.00008421616,0.00036563622,0.9948143,0.0042234864],"study_design_scores_gemma":[0.000026326394,0.000026002888,0.0036946828,0.00020157322,0.000016824293,0.00021192612,0.00013723594,0.00010892046,0.0003796902,0.0008552636,0.9943129,0.000028616303],"about_ca_topic_score_codex":0.038771145,"about_ca_topic_score_gemma":0.048073098,"teacher_disagreement_score":0.07655325,"about_ca_system_score_codex":0.0029897017,"about_ca_system_score_gemma":0.0053839907,"threshold_uncertainty_score":0.25609612},"labels":[],"label_agreement":null},{"id":"W3088448324","doi":"10.3847/1538-4357/abba24","title":"Clumping in the Winds of Wolf–Rayet Stars","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Stars; Instability; Hydrostatic equilibrium; Line (geometry); Spectral line; O-type star; Instability strip","score_opus":0.017627205847479385,"score_gpt":0.23163844867080932,"score_spread":0.21401124282332995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3088448324","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995987,0.00003734226,0.00015055446,0.00000353619,0.0000012317346,0.0000012530421,0.00006050539,0.0000042193533,0.00014276046],"genre_scores_gemma":[0.9996692,0.000007975633,0.00012121112,0.000003719087,0.0000018481218,0.0000011694884,0.00012280459,0.0000016047974,0.000070442096],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998795,0.000015490592,0.000012324937,0.000044917182,0.000024116514,0.000023764893],"domain_scores_gemma":[0.9993789,0.00008478317,0.00025406358,0.000057329104,0.000081781116,0.00014308751],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027157788,0.00017301973,0.00023388235,0.0007043727,0.00023783384,0.0004974996,0.00015941652,0.00023339162,0.00071452593],"category_scores_gemma":[0.0005340801,0.00011759985,0.000181918,0.0004675069,0.00017306245,0.0002732143,0.0003599066,0.00022267693,0.00022623519],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013881871,0.000019316303,0.9489159,0.000012673185,0.000040968025,0.00015020651,0.000114737806,0.00022597492,0.048303936,0.000048641643,0.00003637259,0.001992486],"study_design_scores_gemma":[0.0000024210074,0.00004626901,0.99711657,0.0000020934656,0.0000048915626,0.00013962176,0.000081240134,0.0004715323,0.0019954806,0.000041444633,0.0000956497,0.0000028480363],"about_ca_topic_score_codex":0.0005915747,"about_ca_topic_score_gemma":0.0010540461,"teacher_disagreement_score":0.00071452593,"about_ca_system_score_codex":0.00013409164,"about_ca_system_score_gemma":0.000046278565,"threshold_uncertainty_score":0.0023903847},"labels":[],"label_agreement":null},{"id":"W3088628734","doi":"10.3847/1538-4357/abbc13","title":"Cosmological Insights into the Early Accretion of r-process-enhanced Stars. I. A Comprehensive Chemodynamical Analysis of LAMOST J1109+0754","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; LAMOST; Population; Galaxy; Planet; Abundance of the chemical elements; Abundance (ecology); Galaxy formation and evolution","score_opus":0.014140297720002108,"score_gpt":0.24123305049283283,"score_spread":0.22709275277283072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3088628734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986362,0.00011431491,0.00027063023,0.000044521894,9.981626e-7,0.00000386712,0.00015851481,0.000020787484,0.0007502674],"genre_scores_gemma":[0.9990632,0.000072506424,0.00037318908,0.000013491672,0.0000035636126,0.0000032814855,0.0002849868,0.000015417983,0.00017038335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995184,0.000009462283,0.0000026502764,0.000013620088,0.000010514826,0.000011961197],"domain_scores_gemma":[0.99981433,0.00002442861,0.0000680668,0.00001560864,0.00001597108,0.00006157291],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014340693,0.0002767024,0.00028979898,0.0010828483,0.00028754628,0.00058032316,0.0003780763,0.00021076588,0.0007975697],"category_scores_gemma":[0.00041004055,0.0002304753,0.00038837275,0.00065903214,0.00029823612,0.00036759427,0.00084370404,0.00024324887,0.0001522139],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016404378,0.00009287276,0.9167967,0.00006324499,0.00018440877,0.0011774994,0.0005812771,0.01811225,0.048484255,0.0021823123,0.00043137278,0.011729697],"study_design_scores_gemma":[0.000009820425,0.00004051851,0.9663608,0.0000071007053,0.000033126395,0.00021018872,0.00029348404,0.030336734,0.0011475193,0.00047578412,0.0010673796,0.00001749188],"about_ca_topic_score_codex":0.010375881,"about_ca_topic_score_gemma":0.013542369,"teacher_disagreement_score":0.010375881,"about_ca_system_score_codex":0.0008430552,"about_ca_system_score_gemma":0.0002565222,"threshold_uncertainty_score":0.020631015},"labels":[],"label_agreement":null},{"id":"W3088968998","doi":"10.3847/1538-4357/abb81d","title":"Cloud Atlas: Unraveling the Vertical Cloud Structure with the Time-series Spectrophotometry of an Unusually Red Brown Dwarf","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Brown dwarf; Exoplanet; Wavelength; Planet; Atmospheric model; Spectral line; Atmospheric models; Molecular cloud","score_opus":0.007415344600314973,"score_gpt":0.20836721114271725,"score_spread":0.20095186654240227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3088968998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932099,0.00005431757,0.00393953,0.0000357624,0.000005968978,0.000006741778,0.0018710284,0.0002285706,0.0006482448],"genre_scores_gemma":[0.9944616,0.000026263699,0.0038911428,0.0000060418834,0.0000071628806,0.000004417331,0.0014688814,0.000024382553,0.000110104666],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999471,0.0000074149643,0.0000031207467,0.000018185847,0.00001275606,0.0000114802615],"domain_scores_gemma":[0.9998053,0.000024497771,0.000058033496,0.00004605746,0.000033338547,0.000032736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021250812,0.00017362509,0.00012958572,0.0007850384,0.0002206436,0.00029116872,0.00021905552,0.00012338022,0.00032985982],"category_scores_gemma":[0.0003233477,0.00008419636,0.00026668655,0.00067027356,0.00009130931,0.0003217784,0.000232546,0.00013585434,0.00009443541],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018662085,0.00010141755,0.87444675,0.000038966537,0.0001428243,0.00020254332,0.0001754199,0.036220443,0.050678056,0.0015169578,0.0023102085,0.033979833],"study_design_scores_gemma":[0.000017766426,0.000050834984,0.7774242,0.000005565266,0.000058927282,0.000086356195,0.00007756023,0.21059844,0.008463195,0.00054521987,0.002658164,0.000013745534],"about_ca_topic_score_codex":0.029257407,"about_ca_topic_score_gemma":0.036112398,"teacher_disagreement_score":0.029257407,"about_ca_system_score_codex":0.00041121393,"about_ca_system_score_gemma":0.0003415686,"threshold_uncertainty_score":0.058174253},"labels":[],"label_agreement":null},{"id":"W3089463653","doi":"10.3847/1538-4357/abba3a","title":"ALMaQUEST. IV. The ALMA-MaNGA QUEnching and STar Formation (ALMaQUEST) Survey","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Star formation; Galaxy; Millimeter; Quenching (fluorescence); Observatory; Molecular cloud; Galaxy formation and evolution","score_opus":0.014118235193033896,"score_gpt":0.21923116706941898,"score_spread":0.20511293187638507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3089463653","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.55087715,0.0014643337,0.001621087,0.0014451002,0.00014419392,0.00044934507,0.40892273,0.0019914748,0.03308458],"genre_scores_gemma":[0.60476506,0.00043515014,0.007577152,0.0011444158,0.00044963212,0.00071093335,0.3579616,0.00044762087,0.026508357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997472,0.000048730097,0.00000926028,0.0000842894,0.000052703672,0.000057836365],"domain_scores_gemma":[0.99907047,0.000058753263,0.0002771643,0.000110961075,0.00015086244,0.00033186525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005062372,0.00029006955,0.00020577066,0.001415,0.00033284217,0.0005159803,0.0005612631,0.00027449132,0.010531495],"category_scores_gemma":[0.000649714,0.00016529414,0.0002429925,0.0010662575,0.000120374985,0.00038818415,0.00077643176,0.00026441476,0.004636031],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00070948876,0.00023484352,0.74405825,0.00025030848,0.00015731565,0.00033985006,0.00030576662,0.00050276134,0.007957609,0.0011221948,0.16377252,0.080589056],"study_design_scores_gemma":[0.00012716814,0.00012371912,0.8959908,0.000032624892,0.000026103226,0.00020472925,0.00013822691,0.0010656609,0.000918403,0.00033794955,0.1010189,0.00001570126],"about_ca_topic_score_codex":0.021232612,"about_ca_topic_score_gemma":0.023696944,"teacher_disagreement_score":0.021232612,"about_ca_system_score_codex":0.00048184075,"about_ca_system_score_gemma":0.00037277094,"threshold_uncertainty_score":0.04221803},"labels":[],"label_agreement":null},{"id":"W3089605122","doi":"10.3847/1538-4357/abc014","title":"IQ Collaboratory. II. The Quiescent Fraction of Isolated, Low-mass Galaxies across Simulations and Observations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Yale University","keywords":"Galaxy; Star formation; Galaxy formation and evolution; Stellar mass; Parameter space; Noise (video); Quenching (fluorescence); Stars; Field (mathematics)","score_opus":0.010673043690753439,"score_gpt":0.23837767944264138,"score_spread":0.22770463575188793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3089605122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9018617,0.0003471736,0.03458959,0.00088917726,0.00021730668,0.00022437947,0.015775142,0.008761176,0.037334453],"genre_scores_gemma":[0.95744145,0.00007378064,0.02842664,0.00032225566,0.000033471297,0.0001906105,0.010219799,0.0010374537,0.0022545343],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99954236,0.00016484772,0.000021505579,0.00014329719,0.000067034576,0.000060995524],"domain_scores_gemma":[0.9971546,0.0012171437,0.00021326149,0.00076072756,0.00036316918,0.0002911533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019389772,0.00046694351,0.0004874843,0.00042740506,0.00037260677,0.00087566004,0.0015624185,0.00072070304,0.0040426482],"category_scores_gemma":[0.006568299,0.0002706004,0.00047932786,0.00050900946,0.00047780605,0.0008497309,0.00068775186,0.0007077104,0.0010365023],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007729712,0.00043212136,0.08341814,0.000289308,0.00036164882,0.00011977807,0.00030166024,0.8567742,0.006065044,0.010096585,0.021587688,0.019780844],"study_design_scores_gemma":[0.00024881918,0.00016081499,0.008169034,0.000020315692,0.000050131854,0.0000413852,0.00008463274,0.9780602,0.0036046796,0.0035915372,0.0059409696,0.000027442497],"about_ca_topic_score_codex":0.013000211,"about_ca_topic_score_gemma":0.011718611,"teacher_disagreement_score":0.013000211,"about_ca_system_score_codex":0.00095321384,"about_ca_system_score_gemma":0.00082316645,"threshold_uncertainty_score":0.025849104},"labels":[],"label_agreement":null},{"id":"W3089784271","doi":"10.3847/1538-4357/abd720","title":"Reconstructing Masses of Merging Neutron Stars from Stellar r-process Abundance Signatures","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Los Alamos National Laboratory; National Nuclear Security Administration; Natural Sciences and Engineering Research Council of Canada; Laboratory Directed Research and Development; U.S. Department of Energy; University of Alberta; National Science Foundation","keywords":"r-process; Physics; Astrophysics; Stars; Neutron star; Galaxy; Nucleosynthesis; Population; Astronomy","score_opus":0.009703871086840826,"score_gpt":0.23627474892005937,"score_spread":0.22657087783321855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3089784271","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955923,0.000066921515,0.0035759632,0.00000520053,0.0000012894059,0.0000045748952,0.00016929876,0.00004667301,0.0005377784],"genre_scores_gemma":[0.99797493,0.000026814798,0.0017003019,0.000002048467,0.000001633135,0.000002115077,0.00020400138,0.000008607557,0.00007942053],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998808,0.000026368818,0.000012710576,0.000043121618,0.00002296948,0.000013934392],"domain_scores_gemma":[0.9994215,0.00012087348,0.00021849133,0.000087206165,0.000082873274,0.000069008915],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005509631,0.0003831707,0.0002397344,0.0014662482,0.00017735323,0.0005798648,0.0003002529,0.00028350443,0.00060208375],"category_scores_gemma":[0.0013797429,0.00026076433,0.00028988157,0.00053986645,0.00014782858,0.00038437836,0.0005493899,0.00015913753,0.00037735034],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023529613,0.000024210156,0.9061256,0.00003132101,0.00008430084,0.000081770086,0.00009393915,0.008724402,0.07017841,0.0007729052,0.00006814843,0.01357969],"study_design_scores_gemma":[0.000014896618,0.00012166844,0.7901218,0.000017514298,0.0001010712,0.00033741814,0.0002390468,0.15748465,0.04975319,0.0009883046,0.000798644,0.000021728118],"about_ca_topic_score_codex":0.001020936,"about_ca_topic_score_gemma":0.0011252027,"teacher_disagreement_score":0.0014662482,"about_ca_system_score_codex":0.0002315292,"about_ca_system_score_gemma":0.00011696907,"threshold_uncertainty_score":0.0029138327},"labels":[],"label_agreement":null},{"id":"W3090276904","doi":"10.3847/1538-4357/abba37","title":"Dust Attenuation Curves at z ∼ 0.8 from LEGA-C: Precise Constraints on the Slope and 2175Å Bump Strength","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Canadian Space Agency; European Commission","keywords":"Attenuation; Galaxy; Milky Way; Photometry (optics); Spectral slope; Spectral line; Light curve","score_opus":0.014625699471113352,"score_gpt":0.21149996719701808,"score_spread":0.19687426772590472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3090276904","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99041754,0.0002110033,0.0018302769,0.000029568133,0.000005316843,0.000016056976,0.0029627169,0.00034595578,0.0041814744],"genre_scores_gemma":[0.99345773,0.00004767825,0.0017260641,0.000034498786,0.000012731994,0.000013533053,0.004405619,0.00004152745,0.00026051252],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974877,0.000028170898,0.000012189842,0.000070475726,0.00007510671,0.000065334476],"domain_scores_gemma":[0.9986966,0.00019182642,0.0004294977,0.00021339848,0.0001869567,0.00028169996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042903953,0.0004945172,0.00033971202,0.0034061184,0.00031763868,0.0010126609,0.0004106025,0.0003843837,0.0014899443],"category_scores_gemma":[0.001095609,0.00026928628,0.00036160092,0.0013609547,0.00021248867,0.000241844,0.00064391876,0.00021934583,0.00090926606],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029087532,0.00006994082,0.9253116,0.000053451684,0.00014846177,0.00019856756,0.00022697747,0.0011823954,0.043845862,0.0002493987,0.0010925238,0.027329823],"study_design_scores_gemma":[0.000008009359,0.00001874471,0.9952076,0.0000066794896,0.000021497637,0.00006858779,0.000024763056,0.0019427527,0.001922754,0.00006869115,0.00070360635,0.000006175763],"about_ca_topic_score_codex":0.008193697,"about_ca_topic_score_gemma":0.013143655,"teacher_disagreement_score":0.008193697,"about_ca_system_score_codex":0.00047838117,"about_ca_system_score_gemma":0.0001551348,"threshold_uncertainty_score":0.016292036},"labels":[],"label_agreement":null},{"id":"W3090636479","doi":"10.3847/1538-4357/abbad7","title":"Space Telescope and Optical Reverberation Mapping Project. XII. Broad-line Region Modeling of NGC 5548","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; York University","funders":"Science and Technology Facilities Council; Ministry of Science and ICT, South Korea; Nuclear Safety and Security Commission; Space Telescope Science Institute; Pennsylvania State University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Pennsylvania Space Grant Consortium; National Aeronautics and Space Administration; National Science Foundation","keywords":"Reverberation mapping; Light curve; Parameter space; Active galactic nucleus; Spitzer Space Telescope; Emission spectrum; V band; Kinematics","score_opus":0.039214287368080115,"score_gpt":0.24894550316483346,"score_spread":0.20973121579675336,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3090636479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.82686114,0.00031478002,0.053211737,0.000688265,0.0001239082,0.00020609016,0.075530745,0.012141402,0.030921984],"genre_scores_gemma":[0.90337837,0.000099498204,0.03238774,0.00011906002,0.000049653663,0.00011340565,0.05335638,0.0010428253,0.0094531225],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998555,0.000030204837,0.0000050431686,0.000046742294,0.000033196626,0.00002920164],"domain_scores_gemma":[0.9997603,0.000029856703,0.00003833256,0.00008357228,0.000057027337,0.00003095311],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036681347,0.00041915855,0.0003124046,0.0005875449,0.0002608449,0.0004764625,0.00083873473,0.00038991167,0.006741323],"category_scores_gemma":[0.0009347911,0.00021264025,0.0006125905,0.00052296004,0.00011153412,0.00043647396,0.0003050129,0.00035656657,0.0030832642],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006893539,0.00029990493,0.34782952,0.00013680971,0.00027437304,0.00089844887,0.00068675284,0.40722364,0.015713722,0.006658494,0.09655966,0.123029366],"study_design_scores_gemma":[0.00015827676,0.00014306261,0.1751816,0.000028362094,0.000046788664,0.00025814536,0.00019234186,0.76470536,0.0057185823,0.0044823494,0.049037836,0.000047432837],"about_ca_topic_score_codex":0.037238207,"about_ca_topic_score_gemma":0.02993802,"teacher_disagreement_score":0.037238207,"about_ca_system_score_codex":0.000659094,"about_ca_system_score_gemma":0.00030134406,"threshold_uncertainty_score":0.07404292},"labels":[],"label_agreement":null},{"id":"W3090903084","doi":"10.3847/1538-4357/ac0b44","title":"Quantifying the Impact of the Large Magellanic Cloud on the Structure of the Milky Way’s Dark Matter Halo Using Basis Function Expansions","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":122,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Halo; Astrophysics; Milky Way; Large Magellanic Cloud; Galaxy; Dark matter halo; Dark matter; Galactic halo; Halo mass function; Astronomy","score_opus":0.015796972153484905,"score_gpt":0.24261972068061863,"score_spread":0.22682274852713372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3090903084","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99653083,0.000023046168,0.0024325326,0.000051627198,0.000003829883,0.000004339503,0.000044404012,0.000026641175,0.00088290207],"genre_scores_gemma":[0.99886715,0.000013338295,0.00094580883,0.000011344662,0.000002300982,0.000004738974,0.000041171606,0.000010866618,0.00010339806],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993134,0.00002526925,0.0000027592794,0.000006916581,0.000013374184,0.0000203902],"domain_scores_gemma":[0.999539,0.00024217798,0.00005663256,0.000055496952,0.000038276958,0.00006846491],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043485386,0.00025355906,0.00023508785,0.00024035669,0.00029685802,0.0005162103,0.00049089576,0.00036165366,0.0007802355],"category_scores_gemma":[0.0014918653,0.00017887831,0.00037643866,0.00019285188,0.00043198408,0.00043830142,0.0004840202,0.00035449734,0.00006745612],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008032676,0.00004119741,0.017282484,0.000016451051,0.00006557543,0.00009168514,0.00006540454,0.9722136,0.0045678155,0.0031656057,0.00017238426,0.0022373546],"study_design_scores_gemma":[0.000010665189,0.000022899623,0.0035094663,0.0000022641393,0.0000059740823,0.000007581838,0.000020080839,0.9952962,0.0005325249,0.00049553794,0.000092753915,0.0000040974496],"about_ca_topic_score_codex":0.0111413235,"about_ca_topic_score_gemma":0.008490721,"teacher_disagreement_score":0.0111413235,"about_ca_system_score_codex":0.0005153656,"about_ca_system_score_gemma":0.00041429815,"threshold_uncertainty_score":0.02215296},"labels":[],"label_agreement":null},{"id":"W3091415580","doi":"10.3847/1538-4357/abbd9d","title":"Closure Traces: Novel Calibration-insensitive Quantities for Radio Astronomy","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Closure (psychology); Amplitude; Polarimetry; Polarization (electrochemistry); Stokes parameters; Physics; Interferometry; Calibration; Remote sensing; Optics; Geology; Chemistry; Scattering","score_opus":0.024642768749316143,"score_gpt":0.23370170246318955,"score_spread":0.2090589337138734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091415580","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.036037933,0.00018018253,0.96096265,0.00008175315,0.00007002087,0.000052843436,0.0003284613,0.00084999285,0.001436226],"genre_scores_gemma":[0.67558986,0.00040132864,0.31917667,0.00011983677,0.00036983832,0.00019826731,0.0012296096,0.0007924606,0.0021221589],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9985979,0.00039539664,0.000096389114,0.00026866526,0.00055837876,0.000083156105],"domain_scores_gemma":[0.99297523,0.0030129103,0.00156845,0.0013091161,0.000818081,0.00031624013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017212548,0.0011175626,0.0005864643,0.0022589455,0.00042184224,0.0022365353,0.001140175,0.00076349924,0.0016044123],"category_scores_gemma":[0.013870318,0.0003257596,0.00045251683,0.0017945076,0.0020186326,0.0036182252,0.0020623489,0.0015971945,0.00057843345],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055568654,0.00028899143,0.007430831,0.00030656494,0.00009146592,0.000604269,0.0005520132,0.10603429,0.06861098,0.4646798,0.0041932203,0.3466519],"study_design_scores_gemma":[0.000027047812,0.00021960995,0.0022335087,0.000050818933,0.000021984348,0.00035517573,0.00007089025,0.71169686,0.020636369,0.25562295,0.008965701,0.000099123405],"about_ca_topic_score_codex":0.0005585188,"about_ca_topic_score_gemma":0.00030622643,"teacher_disagreement_score":0.0022589455,"about_ca_system_score_codex":0.00040262492,"about_ca_system_score_gemma":0.00056169904,"threshold_uncertainty_score":0.009102941},"labels":[],"label_agreement":null},{"id":"W3091536308","doi":"10.3847/1538-4357/abbb94","title":"ALMA and VLA Observations of EX Lupi in Its Quiescent State","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Institutes of Natural Sciences; Deutsche Forschungsgemeinschaft; National Astronomical Observatory of Japan; European Commission; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Circumstellar disk; Stars; Radiative transfer; RADIUS; Millimeter; Submillimeter Array; Accretion (finance); Thermal emission; Accretion disc","score_opus":0.030423263500645503,"score_gpt":0.2452993939710209,"score_spread":0.2148761304703754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091536308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988864,0.000018284834,0.000120593744,0.000011819601,0.0000012781982,0.000002090183,0.00015402846,0.00002263848,0.00078288716],"genre_scores_gemma":[0.99949193,0.000006257472,0.00014081523,0.0000052737287,0.0000024772337,0.0000021217613,0.00023110228,0.0000022031334,0.00011781778],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999411,0.000007944972,0.0000026140588,0.000020953525,0.000010509259,0.000016858608],"domain_scores_gemma":[0.99983275,0.00003312121,0.000050779243,0.000019229197,0.000016968494,0.000047126076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001412227,0.00011502316,0.00014011156,0.00048303846,0.00029838004,0.0003586067,0.00022985776,0.0002468174,0.0010494416],"category_scores_gemma":[0.00032732828,0.000091109876,0.0001473178,0.00027347388,0.0001338853,0.00018196848,0.0002938417,0.00017953242,0.00018866934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031642534,0.00009774367,0.9216367,0.000025741774,0.000040258634,0.00041353403,0.0005700595,0.0014929615,0.06574973,0.00034232516,0.0004946169,0.008819922],"study_design_scores_gemma":[0.0000059111294,0.00004306535,0.99623424,0.0000023483403,0.000008130928,0.00009181992,0.00009583175,0.0020492086,0.00095753366,0.00005642745,0.00045263744,0.0000028754664],"about_ca_topic_score_codex":0.00273277,"about_ca_topic_score_gemma":0.003858194,"teacher_disagreement_score":0.00273277,"about_ca_system_score_codex":0.00028371965,"about_ca_system_score_gemma":0.000049571045,"threshold_uncertainty_score":0.0054336786},"labels":[],"label_agreement":null},{"id":"W3091780353","doi":"10.3847/1538-4357/abd9be","title":"The HectoMAP Redshift Survey: First Data Release","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Japan Society for the Promotion of Science; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ministério da Ciência, Tecnologia e Inovação; Cabinet Office, Government of Japan; Toray Science Foundation; High Energy Accelerator Research Organization; Ohio State University; Japan Science and Technology Agency; U.S. Department of Energy; Smithsonian Institution; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Aeronautics and Space Administration; Ministry of Education, Culture, Sports, Science and Technology; Academia Sinica","keywords":"Redshift; Galaxy; Redshift survey; Weak gravitational lensing; Photometric redshift; Limiting; Limiting magnitude; Stars","score_opus":0.01859717076186649,"score_gpt":0.2371905562434088,"score_spread":0.2185933854815423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091780353","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.013266777,0.0000724768,0.0008222459,0.00012884545,0.000017796998,0.00016058979,0.98011863,0.00095729943,0.004455324],"genre_scores_gemma":[0.016376233,0.00007011426,0.0014758393,0.00006575579,0.000030158413,0.0002734429,0.97808003,0.0002600248,0.0033683004],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9987463,0.00011187122,0.00010038702,0.0001682629,0.0006758411,0.0001974572],"domain_scores_gemma":[0.99509794,0.00041226187,0.0009671949,0.0010294759,0.001955424,0.00053780107],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013571552,0.0008490867,0.00070173724,0.0053797355,0.0005606501,0.0013796011,0.0011245131,0.0005137858,0.017591357],"category_scores_gemma":[0.0035633675,0.0005508938,0.00029313267,0.009206717,0.00024039912,0.00072363246,0.0013857352,0.0007623676,0.019858135],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034439037,0.0001519244,0.060264394,0.00031808193,0.000102047816,0.00016545018,0.00019239324,0.00089923595,0.0014904533,0.0010496869,0.90384716,0.031174798],"study_design_scores_gemma":[0.00019346586,0.000055902532,0.48365617,0.000043030865,0.00003569732,0.00013509442,0.0001413988,0.00061278,0.0014487663,0.00033460115,0.51330477,0.00003838382],"about_ca_topic_score_codex":0.044073775,"about_ca_topic_score_gemma":0.038157467,"teacher_disagreement_score":0.044073775,"about_ca_system_score_codex":0.0011351838,"about_ca_system_score_gemma":0.0014341834,"threshold_uncertainty_score":0.087634444},"labels":[],"label_agreement":null},{"id":"W3091826829","doi":"10.3847/1538-4357/ac2aaa","title":"A Self-Calibrating Halo-Based Group Finder: Application to SDSS","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"","keywords":"Halo; Astrophysics; Physics; Galaxy; Luminosity; Astronomy; Galaxy group; Dark matter; Satellite galaxy; Galactic halo; Dark matter halo; Galaxy formation and evolution","score_opus":0.005499287114190967,"score_gpt":0.20620673941025328,"score_spread":0.20070745229606232,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091826829","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.110597484,0.00030413395,0.64332354,0.00028423252,0.00016530114,0.00044890767,0.015328926,0.22568756,0.0038599572],"genre_scores_gemma":[0.15278502,0.00007329558,0.8256177,0.00012353642,0.00006860778,0.00025365895,0.012172842,0.0063071046,0.0025983038],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99928695,0.00012770534,0.00004875553,0.00022025872,0.000264316,0.00005207203],"domain_scores_gemma":[0.9980506,0.00041399532,0.00020383598,0.00069148524,0.00045363719,0.00018649058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003210689,0.00060578174,0.0007422277,0.0042829704,0.0005723245,0.0008541608,0.0012263679,0.0005376265,0.007237435],"category_scores_gemma":[0.0056313276,0.0005390124,0.00084363815,0.0026110054,0.00029802124,0.0009504108,0.0016909344,0.00062842545,0.0041857385],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056705845,0.00037914596,0.097218156,0.00031458423,0.00062614953,0.0003103824,0.00073243753,0.05251056,0.024225688,0.005102069,0.07270427,0.7453094],"study_design_scores_gemma":[0.00046594988,0.00014852882,0.061363604,0.00004976929,0.00009431086,0.00026273626,0.00020511543,0.8289778,0.027869614,0.015766945,0.064636394,0.00015923756],"about_ca_topic_score_codex":0.0059992694,"about_ca_topic_score_gemma":0.0052384017,"teacher_disagreement_score":0.007237435,"about_ca_system_score_codex":0.0006314405,"about_ca_system_score_gemma":0.0006644647,"threshold_uncertainty_score":0.024211645},"labels":[],"label_agreement":null},{"id":"W3091978555","doi":"10.3847/1538-4357/abc339","title":"Five New Post-main-sequence Debris Disks with Gaseous Emission","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"University of California, Los Angeles; College of Engineering, Michigan State University; Jet Propulsion Laboratory; European Southern Observatory; Agencia Nacional de Investigación y Desarrollo; National Science Foundation; European Space Agency; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; University of North Carolina at Chapel Hill; California Institute of Technology; W. M. Keck Foundation; Michigan State University; Ministério da Ciência, Tecnologia, Inovações e Comunicações","keywords":"Debris; Debris disk; White dwarf; Planetary system; Accretion (finance); Planet; Infrared excess; Stars; Emission spectrum","score_opus":0.014454651449594659,"score_gpt":0.2403372709468208,"score_spread":0.22588261949722616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3091978555","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917907,0.0001669785,0.00017645817,0.000016778184,0.000007817058,0.000007335831,0.00006169233,0.000009284916,0.00037460902],"genre_scores_gemma":[0.9992353,0.00003503369,0.00029433134,0.000021444726,0.000006845517,0.000003438435,0.00017617064,0.0000018385581,0.00022570397],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978155,0.000010519022,0.000023385684,0.000063240186,0.000048803766,0.00007264843],"domain_scores_gemma":[0.9993814,0.00009536198,0.00014880174,0.00008317977,0.00008305794,0.00020815946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023706928,0.00031489093,0.00026424063,0.0010108718,0.00075987144,0.0010728058,0.0005388845,0.00053242134,0.0008914168],"category_scores_gemma":[0.0005948786,0.0002516415,0.0002675027,0.00038653903,0.000491174,0.00032162844,0.00072986906,0.00026963823,0.0002608091],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005724461,0.00019724715,0.8940383,0.00012335196,0.000095019495,0.009920007,0.0018994114,0.00021366344,0.07530339,0.0003556508,0.00034863403,0.016932856],"study_design_scores_gemma":[0.00003182377,0.0005654271,0.9600953,0.000017056453,0.000051596046,0.017858878,0.00102631,0.0005542687,0.014380998,0.00019646963,0.0052035423,0.00001835266],"about_ca_topic_score_codex":0.0012726985,"about_ca_topic_score_gemma":0.0015957329,"teacher_disagreement_score":0.0012726985,"about_ca_system_score_codex":0.00050028006,"about_ca_system_score_gemma":0.00012481264,"threshold_uncertainty_score":0.0036298037},"labels":[],"label_agreement":null},{"id":"W3092477418","doi":"10.3847/1538-4357/abbf58","title":"When Do Stalled Stars Resume Spinning Down? Advancing Gyrochronology with Ruprecht 147","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":162,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Berkeley National Laboratory; Leibniz-Gemeinschaft; Science Mission Directorate; Smithsonian Astrophysical Observatory; Heliophysics Division; Danmarks Grundforskningsfond; University of Toronto; Weizmann Institute of Science; National Research Foundation; National Energy Research Scientific Computing Center; Stellar Astrophysics Centre; Space Telescope Science Institute; University of Oxford; Pennsylvania State University; National Science Foundation; European Space Agency; University of Pennsylvania; National Aeronautics and Space Administration; European Commission; California Institute of Technology; Smithsonian Institution","keywords":"Stars; Open cluster; Rotation (mathematics); Main sequence; Asteroseismology; Spinning; Stellar rotation; K-type main-sequence star","score_opus":0.010138984564967389,"score_gpt":0.2192525766157169,"score_spread":0.2091135920507495,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3092477418","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9801338,0.0014133373,0.0107871685,0.00047447337,0.000042778378,0.000016808037,0.00024815227,0.00019155507,0.0066920184],"genre_scores_gemma":[0.99505675,0.00022283438,0.0027217283,0.000026808926,0.000025090227,0.0000066596385,0.000118619435,0.000026596696,0.0017948679],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976355,0.000034733326,0.00000872596,0.000100502875,0.000048284346,0.00004428138],"domain_scores_gemma":[0.9995521,0.00008238627,0.00010654248,0.00009605907,0.0000521087,0.00011081074],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00064249994,0.00027022886,0.00025255536,0.001135854,0.0005395149,0.000902699,0.00038045752,0.00018079056,0.0010249184],"category_scores_gemma":[0.0015306008,0.0001564829,0.00018550252,0.0007422988,0.0005438391,0.00087600795,0.0008577569,0.0003556135,0.0003535279],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003630002,0.000042115367,0.8441293,0.00006540203,0.000070867216,0.00072221097,0.0024217158,0.0050936663,0.020185448,0.014684519,0.0029280472,0.109293655],"study_design_scores_gemma":[0.000009890676,0.00008137823,0.9324511,0.000047208458,0.000035540936,0.0005738605,0.0010243276,0.016672907,0.016690763,0.008547028,0.023821076,0.000044904868],"about_ca_topic_score_codex":0.006599162,"about_ca_topic_score_gemma":0.008414672,"teacher_disagreement_score":0.006599162,"about_ca_system_score_codex":0.00074967573,"about_ca_system_score_gemma":0.00032959136,"threshold_uncertainty_score":0.013121486},"labels":[],"label_agreement":null},{"id":"W3092579213","doi":"10.3847/1538-4357/abbdfa","title":"Serendipitous Discovery of Nine White Dwarfs with Gaseous Debris Disks","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Stars; Spectral line; Emission spectrum; Debris; Line (geometry); Infrared","score_opus":0.009875625711775115,"score_gpt":0.20609770151803927,"score_spread":0.19622207580626416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3092579213","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989127,0.00014263664,0.00017209759,0.000014481673,0.0000074925656,0.0000049098844,0.00019262404,0.00001730676,0.00053576194],"genre_scores_gemma":[0.99863404,0.000093917784,0.00028606795,0.0000212777,0.000014616322,0.0000037344469,0.00065133703,0.000003961567,0.0002910091],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996923,0.000018369177,0.00003378335,0.00011857573,0.00006788101,0.00006916381],"domain_scores_gemma":[0.99917704,0.00012252986,0.00025159054,0.000110257366,0.00009094425,0.00024757002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032643703,0.00024895894,0.00027478745,0.0019307791,0.00061109505,0.0008836317,0.0002985408,0.00023521048,0.0009937756],"category_scores_gemma":[0.0007369488,0.00014077808,0.00020542329,0.0006859828,0.00043082662,0.00027747592,0.00064830034,0.00017713386,0.00048422508],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001143797,0.00003623411,0.97732705,0.000022850953,0.00003093285,0.0018633844,0.0002779757,0.000034788158,0.010665526,0.00013698835,0.00024589803,0.009243901],"study_design_scores_gemma":[0.000012252781,0.00011386705,0.98405683,0.000010240218,0.000036978996,0.007945093,0.00034753198,0.00017017184,0.0039365515,0.00012999399,0.0032322365,0.000008184138],"about_ca_topic_score_codex":0.0012803387,"about_ca_topic_score_gemma":0.0016229709,"teacher_disagreement_score":0.0019307791,"about_ca_system_score_codex":0.000272199,"about_ca_system_score_gemma":0.00020528505,"threshold_uncertainty_score":0.0033245683},"labels":[],"label_agreement":null},{"id":"W3092991002","doi":"10.3847/1538-4357/abb810","title":"Misaligned Twin Molecular Outflows from the Class 0 Protostellar Binary System VLA 1623A Unveiled by ALMA","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Ophiuchus; Outflow; Molecular cloud; Binary number; Sky; Amplitude; Serpens; Redshift; Astronomy; Galaxy; Stars; Optics","score_opus":0.0064339164602251605,"score_gpt":0.21606042043947155,"score_spread":0.2096265039792464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3092991002","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992995,0.000054476237,0.00019481397,0.000010249984,0.0000034356137,0.0000013582953,0.000043192256,0.000017489168,0.00037534581],"genre_scores_gemma":[0.9997472,0.000005185741,0.000119619246,0.000006616232,0.0000037627142,8.4463693e-7,0.00006378762,0.000003106533,0.000049868904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999027,0.000009647912,0.0000055442724,0.000027999067,0.000023628809,0.000030456618],"domain_scores_gemma":[0.999665,0.00003439079,0.0001344955,0.000033959896,0.000025109925,0.00010692892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017238095,0.00015584663,0.00026309103,0.0004989245,0.0004885659,0.0007160382,0.00017337529,0.00028334177,0.00080393266],"category_scores_gemma":[0.00039539457,0.00013230677,0.00015571946,0.000431175,0.00024057359,0.00028686938,0.00046785668,0.0002574037,0.00017687226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069466245,0.00010865633,0.8488758,0.00002849974,0.000100219266,0.0027118633,0.00039259042,0.0006940254,0.13630551,0.0005152156,0.0004181976,0.009154635],"study_design_scores_gemma":[0.000012462515,0.000046072473,0.9931064,0.000004843723,0.000019579047,0.00078081235,0.00015964604,0.0023337977,0.0026385046,0.00017185113,0.0007181124,0.000007815491],"about_ca_topic_score_codex":0.00150353,"about_ca_topic_score_gemma":0.002477919,"teacher_disagreement_score":0.00150353,"about_ca_system_score_codex":0.0002914623,"about_ca_system_score_gemma":0.00012733533,"threshold_uncertainty_score":0.0029895306},"labels":[],"label_agreement":null},{"id":"W3093031215","doi":"10.3847/1538-4357/abccc7","title":"Golden Galactic Binaries for LISA: Mass-transferring White Dwarf Black Hole Binaries","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"European Cooperation in Science and Technology","keywords":"Gravitational wave; White dwarf; Interferometry; Binary number; Luminosity; Gravitational-wave observatory; Black hole (networking); Binary black hole","score_opus":0.01779152908537147,"score_gpt":0.30619501419722855,"score_spread":0.2884034851118571,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093031215","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964116,0.00014875329,0.0018079756,0.00014337534,0.0000059309764,0.000003894551,0.0000680685,0.000031925858,0.0013784595],"genre_scores_gemma":[0.9993961,0.000020109463,0.00020740455,0.000011429422,0.000005381342,0.0000016936845,0.000056786375,0.000006832504,0.00029423562],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999378,0.00001289517,0.0000024920187,0.000020255013,0.00001231756,0.000014301925],"domain_scores_gemma":[0.9995159,0.0001462819,0.0001627328,0.000040603856,0.000026622565,0.00010784001],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004152752,0.00023150645,0.0005349786,0.00060374907,0.00090918766,0.0014789454,0.00042856333,0.0005029531,0.0024219954],"category_scores_gemma":[0.0014752952,0.00013590488,0.0002319804,0.00041134353,0.0007828537,0.0007654804,0.00084496517,0.0004170495,0.0003400863],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007010779,0.00022797892,0.76761544,0.000080798454,0.00012551996,0.0012625512,0.0009133161,0.038483802,0.024277693,0.14044498,0.0018954296,0.023971377],"study_design_scores_gemma":[0.000077304074,0.00023111771,0.38381338,0.000027018634,0.00009677581,0.0012726164,0.0007397707,0.54545486,0.0065798583,0.058991928,0.0026553317,0.00006004456],"about_ca_topic_score_codex":0.0023980595,"about_ca_topic_score_gemma":0.002124491,"teacher_disagreement_score":0.0024219954,"about_ca_system_score_codex":0.0009374691,"about_ca_system_score_gemma":0.00029931826,"threshold_uncertainty_score":0.008102417},"labels":[],"label_agreement":null},{"id":"W3093172326","doi":"10.3847/1538-4357/abebd7","title":"LoCuSS: The Splashback Radius of Massive Galaxy Clusters and Its Dependence on Cluster Merger History","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Cluster (spacecraft); Feature (linguistics); Galaxy cluster; Galaxy; Computer science","score_opus":0.009028811028191312,"score_gpt":0.20227505207895216,"score_spread":0.19324624105076085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093172326","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991985,0.0000815273,0.00015577508,0.0000095791975,7.634839e-7,0.0000017884789,0.00028030184,0.000022700196,0.00024919034],"genre_scores_gemma":[0.99964535,0.0000111994505,0.00006542492,0.0000012055584,0.0000019140114,7.319902e-7,0.00023902771,0.0000029682412,0.000032208354],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996043,0.00007713277,0.000030700878,0.00013297728,0.00010511257,0.000049735117],"domain_scores_gemma":[0.9941988,0.0017500282,0.0023827953,0.0005470281,0.0003203973,0.000800973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060138956,0.00017526314,0.0003286632,0.0019375096,0.00026979973,0.00071946374,0.0003890531,0.00026988465,0.0015555093],"category_scores_gemma":[0.004821286,0.00017859865,0.0003301461,0.0007881694,0.00053613837,0.00045284003,0.00075934234,0.00020287897,0.00032095518],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014818051,0.000008668498,0.9936792,0.000012157794,0.000074613155,0.00006469317,0.00009761486,0.0007390451,0.0026604584,0.00007654371,0.000089143265,0.0023496381],"study_design_scores_gemma":[0.0000014557744,0.00001990505,0.99856323,0.0000015459335,0.0000072220755,0.00008427883,0.000037894202,0.0010144623,0.00018024309,0.000036459078,0.00004999154,0.0000033517392],"about_ca_topic_score_codex":0.003261837,"about_ca_topic_score_gemma":0.002718175,"teacher_disagreement_score":0.003261837,"about_ca_system_score_codex":0.00024957044,"about_ca_system_score_gemma":0.0000995159,"threshold_uncertainty_score":0.0064857006},"labels":[],"label_agreement":null},{"id":"W3093183975","doi":"10.3847/1538-4357/abd7f8","title":"The Dragonfly Wide Field Survey. II. Accurate Total Luminosities and Colors of Nearby Massive Galaxies and Implications for the Galaxy Stellar-mass Function","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Stellar mass; Sky; Surface brightness; Photometry (optics); Astronomy; Fundamental plane (elliptical galaxies); Brightness; Surface brightness fluctuation; Luminous infrared galaxy; Star formation; Galaxy group; Disc galaxy; Stars","score_opus":0.010625393096040138,"score_gpt":0.2263373297926317,"score_spread":0.21571193669659156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093183975","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967619,0.00007964236,0.0002329786,0.000022007447,0.0000018550969,0.0000069279363,0.0017534669,0.000009477614,0.001131542],"genre_scores_gemma":[0.99446255,0.000042302832,0.00081690564,0.00001638987,0.000003900237,0.00001083545,0.004054996,0.0000035002367,0.000588601],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998203,0.000027460228,0.0000068233157,0.00008166584,0.000030346084,0.000033387285],"domain_scores_gemma":[0.9996123,0.0000738689,0.00013736189,0.000055670756,0.00003933585,0.00008146203],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026834646,0.00023158173,0.00012511636,0.0013395573,0.00029462128,0.0004087848,0.00028968265,0.00018192963,0.0008396904],"category_scores_gemma":[0.00061982626,0.00013356742,0.00009966566,0.0006292582,0.00027579692,0.0003958113,0.00044817373,0.00013194054,0.00027324972],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054610384,0.000020150519,0.9882811,0.000010447523,0.000025438147,0.00003788473,0.000096768345,0.00022410764,0.0018864551,0.0001256019,0.000744957,0.008492554],"study_design_scores_gemma":[0.000003144345,0.000009890777,0.9985361,0.00000368994,0.0000057047396,0.00003183727,0.00007193605,0.0003756614,0.0003175796,0.000023330684,0.000619099,0.0000021235974],"about_ca_topic_score_codex":0.023533937,"about_ca_topic_score_gemma":0.07418557,"teacher_disagreement_score":0.023533937,"about_ca_system_score_codex":0.00042826252,"about_ca_system_score_gemma":0.00010273038,"threshold_uncertainty_score":0.046793938},"labels":[],"label_agreement":null},{"id":"W3093208015","doi":"10.3847/1538-4357/abc1d7","title":"Can Large-scale Migration Explain the Giant Planet Occurrence Rate?","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Planet; Giant planet; Planetary migration; Gas giant; Formation and evolution of the Solar System; Planetary system; Solar System; Planetary mass; Protoplanetary disk","score_opus":0.01274376077030494,"score_gpt":0.22548313132070016,"score_spread":0.2127393705503952,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093208015","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929006,0.0002460388,0.0052943984,0.00019221425,0.000010977223,0.000004870927,0.0003090495,0.00007801477,0.0009638042],"genre_scores_gemma":[0.9995265,0.000042139516,0.00028228646,0.000006853445,0.000003144047,0.0000019088548,0.00007782322,0.000008729799,0.000050770373],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999169,0.00001709956,0.0000047263875,0.000034731933,0.000010247743,0.000016221607],"domain_scores_gemma":[0.99884015,0.0005191462,0.00031542906,0.00019022016,0.000058867467,0.0000762194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004430385,0.00030394434,0.0002616282,0.00039421415,0.00018571844,0.0005786485,0.0004725059,0.000381275,0.0012793147],"category_scores_gemma":[0.0035665873,0.0001672818,0.00036141876,0.00040287545,0.0003118288,0.00089061656,0.00033125083,0.00030267256,0.00027068556],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012139154,0.000056182053,0.85163593,0.00008677886,0.00012951474,0.00019979315,0.00013389885,0.122323185,0.0074673244,0.0035615503,0.0009293899,0.013355076],"study_design_scores_gemma":[0.000012660141,0.000054596367,0.3965313,0.000022164824,0.00004355152,0.00027387415,0.00017163911,0.589405,0.0026242505,0.009584949,0.0012484081,0.000027662812],"about_ca_topic_score_codex":0.004719164,"about_ca_topic_score_gemma":0.0028851484,"teacher_disagreement_score":0.004719164,"about_ca_system_score_codex":0.00040651904,"about_ca_system_score_gemma":0.00013542183,"threshold_uncertainty_score":0.00938338},"labels":[],"label_agreement":null},{"id":"W3093272642","doi":"10.3847/1538-4357/abc172","title":"Hubble Space Telescope Astrometry of the Metal-poor Visual Binary μ Cassiopeiae: Dynamical Masses, Helium Content, and Age*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Pennsylvania State University","keywords":"Astrometry; Globular cluster; Visual binary; Hubble space telescope; Helium; Binary star; Parallax; Apparent magnitude; Absolute magnitude; Primary (astronomy)","score_opus":0.02040625671018361,"score_gpt":0.24021431257406314,"score_spread":0.21980805586387953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093272642","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99726653,0.00007122032,0.00016643241,0.000023639037,0.0000028764125,0.000004999507,0.0007485331,0.000012372399,0.0017035032],"genre_scores_gemma":[0.99874794,0.000026312708,0.0002937897,0.000005211141,0.000003838191,0.000003215924,0.0005733472,0.0000037196944,0.00034269673],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999219,0.000006615123,0.0000047587773,0.000034338103,0.000019104453,0.000013265564],"domain_scores_gemma":[0.9995715,0.000056648554,0.00012587271,0.00004649409,0.00009772882,0.0001017567],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018581339,0.00016284584,0.00013147233,0.0007491516,0.00042294813,0.00043692876,0.00018192235,0.00015526993,0.0013646849],"category_scores_gemma":[0.0006314715,0.000082066086,0.00008567152,0.00042247228,0.00021046645,0.0002046218,0.00032984721,0.00018853103,0.00032939692],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007367533,0.000016596743,0.9826728,0.00001200837,0.000018120929,0.00012444674,0.00016488119,0.00022378955,0.011689236,0.00019867199,0.00045681678,0.004348841],"study_design_scores_gemma":[0.0000024155372,0.000016371887,0.9981318,0.0000020908562,0.000004495292,0.00008284814,0.000029895356,0.0003966537,0.0008102101,0.000028115064,0.0004936334,0.0000014871266],"about_ca_topic_score_codex":0.019073311,"about_ca_topic_score_gemma":0.02215962,"teacher_disagreement_score":0.019073311,"about_ca_system_score_codex":0.00052315026,"about_ca_system_score_gemma":0.00021263905,"threshold_uncertainty_score":0.037924588},"labels":[],"label_agreement":null},{"id":"W3093401757","doi":"10.3847/1538-4357/abe626","title":"An Analysis Pipeline for CHIME/FRB Full-array Baseband Data","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Baseband; Pipeline (software); Faraday effect; Pulsar; Microsecond; Ranging; Antenna (radio); Data acquisition","score_opus":0.0253489691095891,"score_gpt":0.36201437506595047,"score_spread":0.33666540595636135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093401757","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.014923879,0.0002342312,0.64727277,0.00032513984,0.00016686307,0.0009066474,0.030061,0.30167058,0.0044389307],"genre_scores_gemma":[0.10529951,0.00025506873,0.7843402,0.00040697915,0.0001383291,0.0015916785,0.07802086,0.020112451,0.0098348595],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99879336,0.00007360398,0.000094984476,0.00035515387,0.0005369846,0.00014588163],"domain_scores_gemma":[0.99701166,0.00057203695,0.00022628978,0.0006224046,0.0013608705,0.00020668548],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015117503,0.0018501264,0.00073197996,0.003858011,0.0010777151,0.0024903456,0.0016439846,0.0006672846,0.016477045],"category_scores_gemma":[0.0054692277,0.00084253517,0.0012454368,0.0025120906,0.0004612733,0.0015492071,0.001770524,0.0012242736,0.019166194],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013213303,0.00039890353,0.01662252,0.00066618883,0.00047365704,0.0016843426,0.0010940761,0.011946684,0.19969855,0.004771007,0.18513301,0.57618976],"study_design_scores_gemma":[0.0003864647,0.00041839475,0.05814977,0.00016738685,0.00021066556,0.000946625,0.00080207194,0.41940892,0.25650772,0.014549291,0.24792373,0.00052887376],"about_ca_topic_score_codex":0.0131784165,"about_ca_topic_score_gemma":0.010416352,"teacher_disagreement_score":0.016477045,"about_ca_system_score_codex":0.0011454113,"about_ca_system_score_gemma":0.0021039296,"threshold_uncertainty_score":0.055121243},"labels":[],"label_agreement":null},{"id":"W3093445122","doi":"10.3847/1538-4357/abc694","title":"The Maximum Energy of Shock-accelerated Electrons in a Microturbulent Magnetic Field","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Toronto Metropolitan University","funders":"Japan Society for the Promotion of Science; National Aeronautics and Space Administration","keywords":"Physics; Electron; Shock (circulatory); Monte Carlo method; Computational physics; Microturbulence; Markov chain Monte Carlo; Acceleration; Magnetic field; Population; Position and momentum space; Momentum (technical analysis); Fermi acceleration; Turbulence; Particle acceleration; Mechanics; Classical mechanics; Quantum mechanics; Statistics","score_opus":0.006161501451392769,"score_gpt":0.20817022649938674,"score_spread":0.20200872504799397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093445122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938816,0.00004456806,0.005033533,0.00006647478,0.0000053240333,0.0000064771325,0.000050794355,0.000044288165,0.00086688827],"genre_scores_gemma":[0.9991829,0.000009869557,0.0006529553,0.000006475231,0.0000013940643,0.000004214325,0.000027620315,0.000006363253,0.00010820878],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989665,0.000028143351,0.0000047943513,0.00001762762,0.000017684533,0.00003521954],"domain_scores_gemma":[0.9989316,0.0006657993,0.00010751837,0.00006993298,0.00011003829,0.00011512046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000674634,0.00016111122,0.00028859984,0.00048845646,0.0005322704,0.0007715403,0.0005439413,0.0005387489,0.0011227801],"category_scores_gemma":[0.0027828563,0.0002830013,0.0003319932,0.00031168494,0.00076859246,0.00056670984,0.000502414,0.0005843639,0.00009630258],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025588335,0.000076376804,0.027533581,0.000032230735,0.000068678935,0.00042781304,0.00013112488,0.9505077,0.009241772,0.009369313,0.00024695,0.0021084682],"study_design_scores_gemma":[0.000031181706,0.00006447624,0.0086335065,0.000011528049,0.0000136884355,0.00006375936,0.0000658104,0.98372895,0.0041603516,0.003068779,0.0001412971,0.000016740598],"about_ca_topic_score_codex":0.00372688,"about_ca_topic_score_gemma":0.0022515357,"teacher_disagreement_score":0.00372688,"about_ca_system_score_codex":0.0007448143,"about_ca_system_score_gemma":0.00038742405,"threshold_uncertainty_score":0.0074103475},"labels":[],"label_agreement":null},{"id":"W3093694080","doi":"10.3847/1538-4357/abda3d","title":"Reconciling EHT and Gas-dynamics Measurements in M87: Is the Jet Misaligned at Parsec Scales?","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Jet (fluid); Angular momentum; Parsec; Telescope; Momentum (technical analysis); Event (particle physics); Stellar mass; Black hole (networking)","score_opus":0.02891555478031595,"score_gpt":0.24369535921681854,"score_spread":0.21477980443650257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093694080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928555,0.00036178896,0.0046005454,0.0001747746,0.000017081918,0.0000037934724,0.0002834633,0.00011455977,0.0015886131],"genre_scores_gemma":[0.9991543,0.000031443677,0.0005598369,0.000030922525,0.000010384333,0.0000022382178,0.00013749092,0.00001602146,0.00005728758],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969685,0.00006074255,0.000025297319,0.00006695267,0.000086467204,0.00006365157],"domain_scores_gemma":[0.9988391,0.0003065055,0.00039784092,0.00018069016,0.00015984173,0.00011614125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011179828,0.00023725224,0.0003999807,0.0008352096,0.00027593446,0.00076755974,0.00054925925,0.0003314603,0.00071428635],"category_scores_gemma":[0.0025943604,0.00019418076,0.00020386114,0.00062308717,0.00047387212,0.0006660371,0.0009729901,0.0004333798,0.0003063526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032140323,0.000040817922,0.9196813,0.000085966356,0.00016553297,0.00078439567,0.00038430555,0.0059805918,0.050712798,0.0028649992,0.0007178246,0.01826014],"study_design_scores_gemma":[0.000014680955,0.00003506178,0.9702369,0.00002215169,0.000052885745,0.0002118024,0.00020121322,0.01979365,0.0070454744,0.0010886195,0.0012855884,0.000011989688],"about_ca_topic_score_codex":0.0023191706,"about_ca_topic_score_gemma":0.0025795775,"teacher_disagreement_score":0.0023191706,"about_ca_system_score_codex":0.0005725084,"about_ca_system_score_gemma":0.00014747998,"threshold_uncertainty_score":0.0059125423},"labels":[],"label_agreement":null},{"id":"W3093798984","doi":"10.3847/1538-4357/abc262","title":"A Characterization of the Circumstellar Gas of WD 1124−293 Using Cloudy","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Astrophysics; Planetesimal; Physics; Photosphere; Planet; White dwarf; Sublimation (psychology); Spectral line; Astronomy; Stars","score_opus":0.013914979636997013,"score_gpt":0.22146363649993156,"score_spread":0.20754865686293456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093798984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986966,0.00002891206,0.0003135011,0.0000108217355,0.000001425605,0.000005989773,0.00046617002,0.00004232547,0.00043417737],"genre_scores_gemma":[0.9989405,0.000011184929,0.00041131792,0.000007022617,0.0000017705414,0.0000032746339,0.00056017254,0.000007697632,0.000057066718],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.0000043753544,0.0000040155714,0.000025868256,0.000012016944,0.000016229507],"domain_scores_gemma":[0.99985754,0.000018326069,0.000036881647,0.00001885299,0.000017444218,0.000050992672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013992064,0.00026746676,0.00017663866,0.0009024036,0.00047840853,0.0003996184,0.0003672237,0.00025155587,0.0008462915],"category_scores_gemma":[0.0002013216,0.00015173368,0.00031157353,0.0006664009,0.00015432452,0.00022642725,0.0003209726,0.00015989621,0.00015726611],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032283043,0.000085628635,0.8661844,0.00003713079,0.000096396594,0.00044930467,0.0002544561,0.0050717425,0.118084475,0.00023727259,0.00036945546,0.008806986],"study_design_scores_gemma":[0.000018725093,0.000057390112,0.97079283,0.0000042863003,0.000032400963,0.00012224217,0.00011849553,0.02106604,0.0070468597,0.000101681355,0.0006311122,0.000007980676],"about_ca_topic_score_codex":0.022103848,"about_ca_topic_score_gemma":0.023616176,"teacher_disagreement_score":0.022103848,"about_ca_system_score_codex":0.000466893,"about_ca_system_score_gemma":0.00010837284,"threshold_uncertainty_score":0.04395038},"labels":[],"label_agreement":null},{"id":"W3093863376","doi":"10.3847/1538-4357/abc016","title":"Herschel Gould Belt Survey Observations of Dense Cores in the Cepheus Flare Clouds","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Victoria; University of Toronto; Herzberg Institute of Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Physics; Astrophysics; Spire (mollusc); Protostar; Molecular cloud; Initial mass function; Star formation; Astronomy; Stars","score_opus":0.054817658455774236,"score_gpt":0.27126097212444367,"score_spread":0.21644331366866942,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093863376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974596,0.00007556957,0.00013695618,0.000037194146,0.0000014530909,0.0000052708765,0.0010252326,0.000039991763,0.0012187539],"genre_scores_gemma":[0.9981812,0.000026882131,0.00035430363,0.000021562118,0.0000042925803,0.0000031450506,0.0012232402,0.000004692766,0.00018059698],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986017,0.000012704691,0.0000047784833,0.000031975524,0.00004869379,0.000041615225],"domain_scores_gemma":[0.9996525,0.0000402716,0.00009753153,0.000047908252,0.000059283833,0.00010255928],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027074595,0.000118512704,0.0001507132,0.0014471966,0.00024739132,0.0002810905,0.00018990836,0.00016729535,0.001179402],"category_scores_gemma":[0.0005011674,0.000119402815,0.00010776217,0.0006703345,0.00013520224,0.0002128557,0.00039314208,0.00011811929,0.00021628241],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001228768,0.000046476132,0.9549217,0.000021088284,0.000064662105,0.00013230542,0.00026277517,0.00086653477,0.021385863,0.00043036576,0.0030478544,0.018697552],"study_design_scores_gemma":[0.0000066369644,0.000005359197,0.99851674,0.0000023008417,0.0000031288314,0.000019702651,0.000023017978,0.00038165422,0.00044268736,0.000028970082,0.0005677276,0.0000020207747],"about_ca_topic_score_codex":0.017926099,"about_ca_topic_score_gemma":0.05555095,"teacher_disagreement_score":0.017926099,"about_ca_system_score_codex":0.0005412416,"about_ca_system_score_gemma":0.00013964366,"threshold_uncertainty_score":0.035643518},"labels":[],"label_agreement":null},{"id":"W3093938602","doi":"10.3847/1538-4357/abd7f5","title":"The Young Supernova Experiment: Survey Goals, Overview, and Operations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":103,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Planetary Science Division; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Stockholms Universitet; Queen's University; Hong Kong Government; Canada Research Chairs; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; Science Mission Directorate; University of Toronto; National Research Foundation; National Centre for Supercomputing Applications; Natural Sciences and Engineering Research Council of Canada; Durham University; Northwestern University; National Central University; Villum Fonden; Los Alamos National Laboratory; University of Washington; Johns Hopkins University; National Science Foundation; Gordon and Betty Moore Foundation; Queen's University Belfast; Canadian Institute for Advanced Research; Nuclear Safety and Security Commission; Space Telescope Science Institute; W. M. Keck Foundation; European Commission; California Institute of Technology; Smithsonian Institution","keywords":"Supernova; Observatory; Light curve; Sky; Cosmology; Dark energy; Night sky","score_opus":0.02221485717391543,"score_gpt":0.26750039878815735,"score_spread":0.2452855416142419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093938602","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.33793524,0.020107495,0.20393594,0.0135930125,0.00059738796,0.011121492,0.31967115,0.008861981,0.084176265],"genre_scores_gemma":[0.34970573,0.009949712,0.25905907,0.0020291556,0.000678414,0.0072494466,0.359589,0.0011540325,0.0105854655],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.99588805,0.0013327837,0.00041322046,0.0007437663,0.0011288854,0.00049321563],"domain_scores_gemma":[0.992044,0.0006887827,0.0011738973,0.0011021888,0.0030029023,0.0019882831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.019226497,0.0010930472,0.00060258666,0.0050234585,0.0006049812,0.003456395,0.0014314306,0.0007808495,0.0022804488],"category_scores_gemma":[0.006616888,0.0007231171,0.0004496355,0.006515017,0.0005644484,0.0029558854,0.0028993478,0.00075204775,0.0030553364],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014328992,0.00048343837,0.6801843,0.00067592534,0.00024583488,0.00013965978,0.00034709292,0.0058652572,0.0047915094,0.011097159,0.088666074,0.20607083],"study_design_scores_gemma":[0.00036093453,0.001218692,0.5442867,0.00084246154,0.00017605849,0.00062295917,0.0010483323,0.023768635,0.0051098703,0.011438183,0.41093126,0.0001959117],"about_ca_topic_score_codex":0.017075935,"about_ca_topic_score_gemma":0.013487461,"teacher_disagreement_score":0.019226497,"about_ca_system_score_codex":0.0015736454,"about_ca_system_score_gemma":0.005008024,"threshold_uncertainty_score":0.10168064},"labels":[],"label_agreement":null},{"id":"W3093950005","doi":"10.3847/1538-4357/abc4e6","title":"Ubiquitous Molecular Outflows in z &gt; 4 Massive, Dusty Galaxies. II. Momentum-driven Winds Powered by Star Formation in the Early Universe","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute","keywords":"Outflow; Galaxy; Star formation; Quasar; Active galactic nucleus; Line (geometry); Stars; Galaxy formation and evolution","score_opus":0.0065071581816023875,"score_gpt":0.19320039502764302,"score_spread":0.18669323684604064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3093950005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995478,0.000051208368,0.000046103953,0.000012144231,9.2595764e-7,0.0000016874694,0.00013053716,0.000007187099,0.00020248225],"genre_scores_gemma":[0.99964964,0.00002400518,0.0000424397,0.0000063358084,0.000003137727,0.0000014999117,0.00017663928,0.000001790816,0.00009464419],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997985,0.000017317398,0.00001270616,0.000047053414,0.000031825577,0.000092618284],"domain_scores_gemma":[0.99908245,0.00011023653,0.00045323375,0.00007435334,0.000066858134,0.000213002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025404544,0.00025452426,0.00031203637,0.001902359,0.00033973195,0.00072837446,0.0002923749,0.00032152326,0.0014280853],"category_scores_gemma":[0.00068027386,0.00017137371,0.00024345721,0.00076238974,0.00052536995,0.00038049146,0.0006206417,0.00021283417,0.00037697013],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045457953,0.0000121703715,0.9941041,0.0000050556687,0.0000143421175,0.0000650787,0.00009611114,0.00003124187,0.003965671,0.000043077656,0.000055655684,0.0015621107],"study_design_scores_gemma":[0.0000010552208,0.000014634238,0.9995454,0.0000012417684,0.00000519221,0.000064573105,0.000071003255,0.00004999473,0.00015344091,0.000015204217,0.00007742154,8.302665e-7],"about_ca_topic_score_codex":0.0031052346,"about_ca_topic_score_gemma":0.0034799916,"teacher_disagreement_score":0.0031052346,"about_ca_system_score_codex":0.00020820166,"about_ca_system_score_gemma":0.00009676413,"threshold_uncertainty_score":0.006174326},"labels":[],"label_agreement":null},{"id":"W3094083696","doi":"10.3847/1538-4357/abc417","title":"Supernova 2018cuf: A Type IIP Supernova with a Slow Fall from Plateau","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Supernova; Ejecta; Red supergiant; Photosphere; Photometry (optics); Supergiant; Absolute magnitude; Light curve","score_opus":0.015964445276738334,"score_gpt":0.21625783272219387,"score_spread":0.20029338744545555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094083696","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981786,0.00011765432,0.0005467014,0.00002322241,0.000014809794,0.000014254711,0.00025302186,0.00007004447,0.0007817197],"genre_scores_gemma":[0.99855787,0.000034106142,0.00037606442,0.000021801136,0.000019010864,0.0000073683914,0.00069009146,0.000011519779,0.00028219132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998853,0.000006665611,0.000009343471,0.000036558842,0.000025448495,0.000036588073],"domain_scores_gemma":[0.99969816,0.000023637362,0.00008056643,0.000035217887,0.000038308546,0.00012423076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019470505,0.00057188584,0.00036878648,0.0009212984,0.00058156095,0.00048739577,0.00033386392,0.0005043564,0.0009262802],"category_scores_gemma":[0.0003813286,0.00014694098,0.0004901308,0.00042719938,0.00027399842,0.00022797179,0.00035646293,0.00038754483,0.00022126234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009928143,0.00033834952,0.8402552,0.0000763893,0.00016577831,0.042814914,0.00015889741,0.0016227639,0.085568465,0.0010984401,0.0019779673,0.02493004],"study_design_scores_gemma":[0.000069395865,0.00069155224,0.93644834,0.000027566126,0.000039364906,0.03883747,0.00016347607,0.0064059007,0.01158337,0.0005233619,0.005184224,0.000025942623],"about_ca_topic_score_codex":0.0029310766,"about_ca_topic_score_gemma":0.002218749,"teacher_disagreement_score":0.0029310766,"about_ca_system_score_codex":0.0003069329,"about_ca_system_score_gemma":0.0001526175,"threshold_uncertainty_score":0.0058280826},"labels":[],"label_agreement":null},{"id":"W3094088293","doi":"10.3847/1538-4357/abc47f","title":"Ubiquitous Molecular Outflows in z &gt; 4 Massive, Dusty Galaxies. I. Sample Overview and Clumpy Structure in Molecular Outflows on 500 pc Scales","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute","keywords":"Galaxy; Star formation; Outflow; Population; Molecular cloud; High resolution; Galaxy formation and evolution; Hydrogen molecule","score_opus":0.009013035710844842,"score_gpt":0.2183251769108625,"score_spread":0.20931214120001768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094088293","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99516886,0.0004634616,0.00012122786,0.000042074043,0.0000027127053,0.000025996596,0.0034168432,0.000033278007,0.0007254185],"genre_scores_gemma":[0.9936854,0.00046102217,0.00022700822,0.0000336573,0.000014237812,0.000030676023,0.004962412,0.000014387247,0.00057116523],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995784,0.000031950294,0.000044013264,0.00011494327,0.00006105336,0.00016967955],"domain_scores_gemma":[0.998765,0.00011982777,0.00050167076,0.00010502802,0.00013550931,0.0003729861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034348152,0.00043322556,0.0004176451,0.0050691697,0.0005212941,0.0009157106,0.0005297448,0.00041009078,0.0021674454],"category_scores_gemma":[0.0007359648,0.00024699373,0.00038669418,0.0023920075,0.00056960055,0.00062315987,0.0013528307,0.00022749645,0.00092228426],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007106539,0.00001345385,0.9942834,0.000027483673,0.000024992736,0.00012456722,0.0002296624,0.000024022904,0.001838285,0.000049587943,0.00023657469,0.0030768474],"study_design_scores_gemma":[0.0000014827398,0.000022350974,0.99900913,0.000004351278,0.0000109861585,0.00017684506,0.00017811843,0.00002603703,0.00014563551,0.000011064766,0.00041218378,0.0000016596713],"about_ca_topic_score_codex":0.009339274,"about_ca_topic_score_gemma":0.00981185,"teacher_disagreement_score":0.009339274,"about_ca_system_score_codex":0.0002968416,"about_ca_system_score_gemma":0.00025833378,"threshold_uncertainty_score":0.018569827},"labels":[],"label_agreement":null},{"id":"W3094198337","doi":"10.3847/1538-4357/abc3bf","title":"Fast Outflows in Hot Dust-obscured Galaxies Detected with Keck/NIRES","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Galaxy; Redshift; Active galactic nucleus; Spectral energy distribution; Photometry (optics); Emission spectrum; Spectral line; Star formation","score_opus":0.008672638634890812,"score_gpt":0.1970522500392705,"score_spread":0.18837961140437967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094198337","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99944824,0.000046857436,0.000070067916,0.0000052055175,0.0000011638987,0.0000019494444,0.00013229137,0.000008126938,0.00028603265],"genre_scores_gemma":[0.9991855,0.000037774636,0.00018739978,0.000008387605,0.0000048639663,0.000003061542,0.00038493492,0.0000030136835,0.0001849722],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974424,0.0000342479,0.000022861997,0.000068044246,0.000060681446,0.00006987443],"domain_scores_gemma":[0.99885094,0.00016500066,0.0004715005,0.000088324894,0.0001117295,0.000312522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047881916,0.0003606074,0.00031308678,0.0020507777,0.00031891066,0.000564094,0.00035611715,0.00022202205,0.0011009466],"category_scores_gemma":[0.000855103,0.0002455497,0.00022279352,0.0006046509,0.00028367314,0.00052464183,0.0007935869,0.00017929566,0.00028800612],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013442762,0.000041096675,0.99134916,0.000014510597,0.000047597838,0.00016804015,0.00018236376,0.00016521293,0.0051339236,0.00004509835,0.00009968153,0.002618978],"study_design_scores_gemma":[0.0000034254313,0.00003274736,0.9984084,0.000004367306,0.000012621272,0.00022735055,0.000097791206,0.00024153428,0.00071684225,0.000016696598,0.00023470035,0.0000035300397],"about_ca_topic_score_codex":0.0019804114,"about_ca_topic_score_gemma":0.003574972,"teacher_disagreement_score":0.0020507777,"about_ca_system_score_codex":0.00029500213,"about_ca_system_score_gemma":0.00007293532,"threshold_uncertainty_score":0.003937781},"labels":[],"label_agreement":null},{"id":"W3094306680","doi":"10.3847/1538-4357/abad9e","title":"Anisotropy of Velocity Centroids and the Signature of Different MHD Modes in the Turbulent ISM","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Magnetohydrodynamics; Anisotropy; Turbulence; Centroid; Astrophysics; Signature (topology); Computational physics; Astronomy; Classical mechanics; Mechanics; Plasma; Optics; Geometry; Nuclear physics","score_opus":0.009839140476370578,"score_gpt":0.21818744427620845,"score_spread":0.20834830379983788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094306680","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99613154,0.0000593085,0.0026150576,0.000074289215,0.00000702887,0.0000054123016,0.0000960713,0.00011725738,0.0008940891],"genre_scores_gemma":[0.9994771,0.000009993429,0.00042775803,0.0000020270227,0.0000021211777,0.0000012526268,0.000034741795,0.0000105978515,0.000034408764],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990845,0.000020989377,0.0000059873373,0.00001893874,0.0000189781,0.000026676362],"domain_scores_gemma":[0.99946076,0.000168277,0.00013841665,0.00006151992,0.000078418634,0.00009258983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034173718,0.00036006395,0.00024215618,0.00063298334,0.00035713555,0.000864551,0.00025607843,0.00030786838,0.0006452033],"category_scores_gemma":[0.0014685764,0.0003097535,0.00030580777,0.00037519995,0.0005707543,0.0004296674,0.0004242538,0.0004045943,0.00008587126],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012139232,0.00029654556,0.12849164,0.00009991162,0.00016236011,0.00045463294,0.00043905515,0.6344535,0.21048109,0.01305388,0.0009634001,0.009890095],"study_design_scores_gemma":[0.00009641329,0.00007026201,0.07908739,0.000011164918,0.000021128715,0.000064828906,0.00006978101,0.9043056,0.013969705,0.0019146436,0.0003425543,0.00004654592],"about_ca_topic_score_codex":0.003556953,"about_ca_topic_score_gemma":0.0012800113,"teacher_disagreement_score":0.003556953,"about_ca_system_score_codex":0.00057606737,"about_ca_system_score_gemma":0.00021690485,"threshold_uncertainty_score":0.0070725083},"labels":[],"label_agreement":null},{"id":"W3094373497","doi":"10.3847/1538-4357/abc6ff","title":"Strong Mg ii and Fe ii Absorbers at 2.2 &lt; z &lt; 6.0","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Key Research and Development Program of China; Chinese Academy of Sciences; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; Strong; National Science Foundation","keywords":"Physics; Astrophysics; Quasar; Redshift; Galaxy; Luminosity; Equivalent width; Spectral line; RADIUS; Wavelength; Emission spectrum; Astronomy; Optics","score_opus":0.0074267059096971896,"score_gpt":0.20828621701103986,"score_spread":0.20085951110134267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094373497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907035,0.000035376142,0.000071341376,0.000013548101,0.0000014125606,0.000002139118,0.00009712388,0.000017693697,0.0006909548],"genre_scores_gemma":[0.9993449,0.000014794936,0.00010189296,0.000009918812,0.0000049205373,0.0000010856497,0.00016038776,0.0000032287187,0.0003587744],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999169,0.0000039777788,0.0000031564257,0.000017540811,0.000024701736,0.000033772125],"domain_scores_gemma":[0.99966943,0.000018094517,0.00014435034,0.000011485396,0.000034927056,0.0001218106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014348298,0.00020845492,0.00018600943,0.00089109363,0.0003962332,0.0005177023,0.00018121772,0.00018979485,0.001924535],"category_scores_gemma":[0.00016732869,0.0001219546,0.00012976205,0.00043687504,0.00022354742,0.00021056419,0.00034868385,0.00023306094,0.00045843542],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003011249,0.00011392641,0.8951659,0.000024282717,0.000038069255,0.0011467927,0.00043097493,0.0001246769,0.094390124,0.00017938906,0.00049940095,0.0075852606],"study_design_scores_gemma":[0.0000017372057,0.000033011063,0.99829406,8.3186626e-7,0.000004420969,0.00011805245,0.00004937108,0.00005320564,0.0011658918,0.000010069601,0.0002676689,0.0000016388442],"about_ca_topic_score_codex":0.0024296874,"about_ca_topic_score_gemma":0.0045448537,"teacher_disagreement_score":0.0024296874,"about_ca_system_score_codex":0.00021912801,"about_ca_system_score_gemma":0.00007556669,"threshold_uncertainty_score":0.0064382553},"labels":[],"label_agreement":null},{"id":"W3094412145","doi":"10.3847/1538-4357/abc484","title":"The Catalogue for Astrophysical Turbulence Simulations (CATS)","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; University of British Columbia; Herzberg Institute of Astrophysics","funders":"Simons Foundation","keywords":"Turbulence; Magnetohydrodynamic turbulence; Magnetohydrodynamic drive; Magnetohydrodynamics; K-epsilon turbulence model; Computational astrophysics; Cosmic ray","score_opus":0.0194707936283027,"score_gpt":0.25776091801805967,"score_spread":0.23829012438975697,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094412145","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.010038992,0.001462942,0.073217474,0.00046478346,0.00041578495,0.00043965632,0.7567099,0.13615791,0.021092579],"genre_scores_gemma":[0.018296054,0.0008902174,0.04000458,0.00030669707,0.00009787867,0.00071130914,0.92325836,0.014115716,0.0023192565],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9984102,0.00022238535,0.00033122112,0.00019480736,0.00069713313,0.00014418074],"domain_scores_gemma":[0.994538,0.0013354302,0.00047097923,0.0017658622,0.0013101198,0.0005796081],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019891749,0.0023393333,0.0016598864,0.00417757,0.0006771465,0.0031468123,0.003973415,0.0017351814,0.019605404],"category_scores_gemma":[0.009571036,0.0010168885,0.002188968,0.0060393414,0.00048054385,0.0024166498,0.0023024366,0.0024470924,0.01991277],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007059789,0.00018835485,0.011199243,0.002450265,0.00049596553,0.00036747227,0.00022034065,0.05536551,0.0037507112,0.029294346,0.82848537,0.06747641],"study_design_scores_gemma":[0.0007340442,0.00007773056,0.0064680167,0.00045354126,0.00011306904,0.00023286178,0.000066805915,0.10546648,0.005080155,0.02320628,0.8579213,0.00017971406],"about_ca_topic_score_codex":0.0076131467,"about_ca_topic_score_gemma":0.0068970546,"teacher_disagreement_score":0.019605404,"about_ca_system_score_codex":0.0009307846,"about_ca_system_score_gemma":0.0026895353,"threshold_uncertainty_score":0.06558657},"labels":[],"label_agreement":null},{"id":"W3094421459","doi":"10.3847/1538-4357/abbeff","title":"A Large Massive Quiescent Galaxy Sample at z ∼ 1.2","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Redshift; Balmer series; Galaxy formation and evolution; Redshift survey; Elliptical galaxy; Sample (material); Lenticular galaxy; Surface brightness fluctuation","score_opus":0.010196987782457008,"score_gpt":0.21375550330662724,"score_spread":0.20355851552417023,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094421459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978672,0.00009457441,0.00042665546,0.00002416815,0.0000017813297,0.000035118203,0.0008370319,0.000027638982,0.0006857249],"genre_scores_gemma":[0.9952205,0.00007403809,0.00074728776,0.000029300412,0.000017526438,0.000027195407,0.0031266399,0.000007906604,0.0007495743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999866,0.000019206596,0.000010024872,0.000040473424,0.000029167322,0.00003512337],"domain_scores_gemma":[0.9997404,0.000032782857,0.00004688495,0.000041078034,0.000028755388,0.00011011069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029696812,0.0001633153,0.00019672586,0.0011810727,0.0003906668,0.00030613857,0.00025697067,0.00013734993,0.00258114],"category_scores_gemma":[0.0004967566,0.00011279092,0.00016461812,0.0007872277,0.00016191314,0.00022109594,0.00046384108,0.00012234818,0.00081184274],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021125602,0.00017715557,0.9543321,0.00002948524,0.000032420372,0.00030723034,0.0005961242,0.00013418942,0.016827466,0.0004300629,0.0014564209,0.025466083],"study_design_scores_gemma":[0.000009654812,0.00005732069,0.9972703,0.0000024195315,0.000009692979,0.00015972239,0.00009789889,0.0002109128,0.00061740645,0.000039478076,0.0015228764,0.0000023976504],"about_ca_topic_score_codex":0.0029050647,"about_ca_topic_score_gemma":0.005857556,"teacher_disagreement_score":0.0029050647,"about_ca_system_score_codex":0.00011277833,"about_ca_system_score_gemma":0.00013901472,"threshold_uncertainty_score":0.008634806},"labels":[],"label_agreement":null},{"id":"W3094610130","doi":"10.3847/1538-4357/abfb66","title":"Relaxation in a Fuzzy Dark Matter Halo. II. Self-consistent Kinetic Equations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Agence Nationale de la Recherche; National Aeronautics and Space Administration","keywords":"Matter wave; Dark matter; Kinetic energy; Dark matter halo; Relaxation (psychology); Distribution function; Cold dark matter; Dispersion relation; Galaxy; Kinetic theory","score_opus":0.008623624213168445,"score_gpt":0.21848441312993722,"score_spread":0.20986078891676876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094610130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75295913,0.0028300043,0.18325531,0.005515626,0.00040214014,0.00017640696,0.0007059038,0.00046438587,0.05369114],"genre_scores_gemma":[0.97214264,0.00049037574,0.009835886,0.00067530305,0.00015373455,0.0000734614,0.00026430358,0.00012223251,0.016242081],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996793,0.00008633534,0.000017253371,0.000040339488,0.000078069366,0.00009873063],"domain_scores_gemma":[0.99871385,0.000344113,0.0002578689,0.00011770708,0.00025031366,0.00031625628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011025002,0.00084131135,0.0011932516,0.0013943658,0.0010958147,0.0021445896,0.0023750826,0.001905809,0.0031533944],"category_scores_gemma":[0.003449418,0.0007402492,0.001477274,0.000680483,0.0036238371,0.002722242,0.0022334727,0.0013949621,0.00036000198],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000113499846,0.00008342792,0.0029479037,0.00011066832,0.00008029714,0.00058306736,0.00025250335,0.5116962,0.0040314975,0.47576055,0.001959093,0.0023812153],"study_design_scores_gemma":[0.000041827614,0.000008058859,0.00047732206,0.00000919326,0.000006091012,0.00005733494,0.00003145407,0.96247536,0.0001634224,0.036437348,0.000269939,0.000022720253],"about_ca_topic_score_codex":0.023680236,"about_ca_topic_score_gemma":0.0061132475,"teacher_disagreement_score":0.023680236,"about_ca_system_score_codex":0.0027587845,"about_ca_system_score_gemma":0.0015122794,"threshold_uncertainty_score":0.04708481},"labels":[],"label_agreement":null},{"id":"W3094636358","doi":"10.3847/1538-4357/ac602e","title":"Secular Dynamics around a Supermassive black hole via Multipole Expansion","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Sorbonne Université; Agence Nationale de la Recherche; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Algorithm; Multipole expansion; Supermassive black hole; Stars; Astrophysics; Computer science; Galaxy; Quantum mechanics","score_opus":0.005285271005325071,"score_gpt":0.20114349347561467,"score_spread":0.19585822247028958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3094636358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6613939,0.00071036315,0.3050121,0.001018504,0.00026845763,0.00008887167,0.0001422692,0.00055599335,0.030809497],"genre_scores_gemma":[0.9584241,0.00031067774,0.032076295,0.00018689965,0.000074793905,0.000059113263,0.000071428214,0.00019936255,0.00859733],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998833,0.000040132734,0.0000035043188,0.000011412332,0.00003505564,0.000026666587],"domain_scores_gemma":[0.9995523,0.00014100246,0.00010232148,0.000050685907,0.00007087385,0.00008276326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047431188,0.000464391,0.0005766417,0.00052446383,0.00056968303,0.00083561125,0.000989312,0.00068757427,0.0035272094],"category_scores_gemma":[0.0013167296,0.00033410208,0.0005266294,0.0002898089,0.0012327554,0.0010259975,0.0011950207,0.00073600304,0.00043273417],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018833508,0.00010873118,0.0038649985,0.00010387697,0.00006164799,0.00056234165,0.00032855652,0.801593,0.009587815,0.17152534,0.0023928164,0.009682537],"study_design_scores_gemma":[0.000008885617,0.00001262902,0.00022780383,0.000004285464,0.0000035856622,0.000013180094,0.000013028281,0.99314594,0.00021408741,0.0058587277,0.00049405615,0.0000037831855],"about_ca_topic_score_codex":0.006594181,"about_ca_topic_score_gemma":0.005683247,"teacher_disagreement_score":0.006594181,"about_ca_system_score_codex":0.0008719898,"about_ca_system_score_gemma":0.000584478,"threshold_uncertainty_score":0.013111591},"labels":[],"label_agreement":null},{"id":"W3095426646","doi":"10.3847/1538-4357/abee15","title":"Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO–Virgo Run O3a","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal","funders":"Division of Human Resource Development; Australian Research Council; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Vlaamse regering; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; Generalitat de Catalunya; Kavli Foundation; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Fundacja na rzecz Nauki Polskiej; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; European Commission; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; European Regional Development Fund; Scottish Universities Physics Alliance; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; Institut des Origines de Lyon; Centres de Recerca de Catalunya; Max-Planck-Gesellschaft; Royal Society; Science and Engineering Research Board; National Science Foundation","keywords":"LIGO; Gravitational wave; Swift; Fermi Gamma-ray Space Telescope; Neutron star; Gamma-ray burst; Population","score_opus":0.00881881939961176,"score_gpt":0.22754766111627758,"score_spread":0.21872884171666582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3095426646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999198,0.00003905414,0.00014687845,0.000013385997,0.0000018263373,0.000005887718,0.0002696903,0.000015193513,0.00031019442],"genre_scores_gemma":[0.99832076,0.00002762113,0.00039846808,0.000013954522,0.0000058244823,0.0000050191843,0.0010804007,0.0000066900916,0.00014109208],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972636,0.000036276462,0.000022445012,0.00006208399,0.00007525947,0.00007766104],"domain_scores_gemma":[0.9984242,0.000252292,0.00069946545,0.00012052713,0.00012408699,0.00037939817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005531779,0.00026315174,0.00027432386,0.0022909564,0.0006176329,0.0007571994,0.0002585992,0.00036079017,0.0008968649],"category_scores_gemma":[0.00094157964,0.00012201473,0.00041375504,0.0011729498,0.0003031488,0.0002453419,0.0006700669,0.0002648924,0.00023199942],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023760859,0.00004270403,0.98616636,0.000010485172,0.00006389437,0.00019677414,0.0001315146,0.00020952274,0.008859209,0.00007418976,0.00016032463,0.0038473783],"study_design_scores_gemma":[0.000005241717,0.00004950121,0.99796486,0.0000037488417,0.000018282082,0.00015035627,0.00009269783,0.0004039938,0.0010456182,0.000026139443,0.00023430989,0.00000525227],"about_ca_topic_score_codex":0.0066828667,"about_ca_topic_score_gemma":0.016755274,"teacher_disagreement_score":0.0066828667,"about_ca_system_score_codex":0.00037762392,"about_ca_system_score_gemma":0.000315442,"threshold_uncertainty_score":0.0132879615},"labels":[],"label_agreement":null},{"id":"W3095678391","doi":"10.3847/1538-4357/abc429","title":"Measuring Dark Matter in Galaxies: The Mass Fraction within Five Effective Radii","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; McMaster University","funders":"","keywords":"Galaxy; Satellite galaxy; Dark matter; Effective radius; RADIUS; Stellar mass; Velocity dispersion; Dark galaxy; Weak gravitational lensing","score_opus":0.008971398823072933,"score_gpt":0.20120884889759505,"score_spread":0.19223745007452211,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3095678391","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99584323,0.00006674943,0.0028829172,0.000020255638,0.0000020812372,0.000006135126,0.0003404679,0.00010187697,0.00073620037],"genre_scores_gemma":[0.99734265,0.000015515372,0.0023138286,0.0000032626992,0.0000013815861,0.0000037420086,0.00024195088,0.000004473049,0.000073080366],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998915,0.00003068862,0.000005597145,0.000028119974,0.000027907714,0.000016176271],"domain_scores_gemma":[0.9995648,0.00016975639,0.00011751349,0.000057796096,0.0000418305,0.0000482573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040764888,0.00018234382,0.000118180134,0.0005485182,0.00011615258,0.00032270653,0.00028237014,0.00014809312,0.0006911811],"category_scores_gemma":[0.00155213,0.00008882865,0.0001687409,0.00046801614,0.00026873304,0.00030005226,0.000309908,0.00013409574,0.00010377126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016364717,0.000082346945,0.8619433,0.000060722243,0.00014902418,0.000056710982,0.0001847564,0.10702374,0.011909333,0.0016968588,0.00064047944,0.016089082],"study_design_scores_gemma":[0.000029995363,0.00020657599,0.7022345,0.000017929353,0.000031765645,0.00012501214,0.00010487437,0.28196526,0.012261501,0.0014806248,0.0015209669,0.000020965954],"about_ca_topic_score_codex":0.005887183,"about_ca_topic_score_gemma":0.007285869,"teacher_disagreement_score":0.005887183,"about_ca_system_score_codex":0.00031207086,"about_ca_system_score_gemma":0.00012867492,"threshold_uncertainty_score":0.011705816},"labels":[],"label_agreement":null},{"id":"W3095691449","doi":"10.3847/1538-4357/abc2cb","title":"Exploring the Perturbed Milky Way Disk and the Substructures of the Outer Disk","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Key Research and Development Program of China; National Natural Science Foundation of China; National Science Foundation","keywords":"Milky Way; Spiral galaxy; Galaxy; Galactic plane; Disc; Galactic Center; Sky; Dwarf galaxy; Stars; Galactic tide","score_opus":0.025661275740152964,"score_gpt":0.20722768900572017,"score_spread":0.18156641326556722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3095691449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99887997,0.00009693346,0.00059222884,0.000025060217,0.000001280149,0.0000012850711,0.000028026767,0.000008375713,0.0003668091],"genre_scores_gemma":[0.99963474,0.000037287413,0.00022939195,0.000003458038,9.978048e-7,5.5619313e-7,0.00001886073,0.0000020470266,0.00007270755],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999727,0.0000074604873,0.0000011743706,0.0000070844085,0.0000045893785,0.0000069732773],"domain_scores_gemma":[0.9998343,0.00006989372,0.00003705753,0.00001593952,0.000013120986,0.000029715371],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099596495,0.00014825434,0.00020129397,0.00032988278,0.00017012657,0.00051960093,0.00031679822,0.00025140028,0.00068393763],"category_scores_gemma":[0.00051885657,0.0001564104,0.00021058065,0.0002826117,0.0003574774,0.0005593046,0.0003172298,0.00017229699,0.00007269112],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006801931,0.00021915125,0.35078353,0.00019056539,0.00047893266,0.0022459005,0.0009356335,0.51221263,0.10486599,0.008639586,0.00051948265,0.018228335],"study_design_scores_gemma":[0.00005009792,0.00019946006,0.31176394,0.000017209519,0.000081488506,0.00033134848,0.00077415333,0.67511535,0.005315482,0.004871812,0.0014488526,0.000030840656],"about_ca_topic_score_codex":0.006490852,"about_ca_topic_score_gemma":0.0039081555,"teacher_disagreement_score":0.006490852,"about_ca_system_score_codex":0.00039935432,"about_ca_system_score_gemma":0.0001448186,"threshold_uncertainty_score":0.012906134},"labels":[],"label_agreement":null},{"id":"W3095777331","doi":"10.3847/1538-4357/abc483","title":"Chandra Observations of Abell 2261 Brightest Cluster Galaxy, a Candidate Host to a Recoiling Black Hole","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Physics; Astrophysics; Galaxy; Black hole (networking); Galaxy cluster; Astronomy; Intermediate-mass black hole; Accretion (finance); Brightest cluster galaxy; Stellar mass; Supermassive black hole; Star formation","score_opus":0.013258047375731255,"score_gpt":0.22285617935262206,"score_spread":0.2095981319768908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3095777331","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966097,0.000104562976,0.00011448697,0.00005347373,0.0000063456914,0.000010137834,0.00073181675,0.000072956005,0.0022966133],"genre_scores_gemma":[0.9975854,0.000055141663,0.00057632796,0.000030150404,0.000012899023,0.0000039633487,0.0008931093,0.000010463855,0.0008325472],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998939,0.000006861249,0.0000050966983,0.000028353996,0.000025950496,0.000039808125],"domain_scores_gemma":[0.99950635,0.0000335152,0.00012715592,0.000047423433,0.000047985377,0.0002376084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016375954,0.00025261028,0.00027120425,0.0012603134,0.000832267,0.00047148732,0.00031140188,0.0002514657,0.0018102429],"category_scores_gemma":[0.0002487492,0.00016856722,0.00020562748,0.00055129617,0.00018286862,0.00019443697,0.00036756432,0.00031636722,0.0006111568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014920423,0.00054156984,0.6341305,0.00018282898,0.00015327534,0.0070037576,0.0011382187,0.001418396,0.32658407,0.00068045984,0.0049896175,0.021685345],"study_design_scores_gemma":[0.000009627858,0.00007202221,0.9925673,0.0000051513375,0.0000167566,0.0007275304,0.000094179464,0.00040607728,0.004598534,0.000033095872,0.0014586975,0.000011004599],"about_ca_topic_score_codex":0.008887579,"about_ca_topic_score_gemma":0.016108217,"teacher_disagreement_score":0.008887579,"about_ca_system_score_codex":0.00043655737,"about_ca_system_score_gemma":0.00015071765,"threshold_uncertainty_score":0.017671704},"labels":[],"label_agreement":null},{"id":"W3096119508","doi":"10.3847/1538-4357/abdab4","title":"Swift Follow-up Observations of Gravitational-wave and High-energy Neutrino Coincident Signals","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Neutrino; Swift; Observatory; Sky; Neutrino astronomy; Neutrino oscillation; Neutrino detector; Solar neutrino problem","score_opus":0.01970264892322804,"score_gpt":0.22480251542016455,"score_spread":0.2050998664969365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3096119508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9910573,0.0002317239,0.0023457368,0.00011830445,0.000062995416,0.000041046787,0.0023353489,0.00021364349,0.0035939317],"genre_scores_gemma":[0.9911863,0.00005619928,0.0032401083,0.00008983994,0.00005142657,0.000026372067,0.004381509,0.00006886979,0.00089939684],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99940026,0.000042077092,0.00004047688,0.00013430236,0.00022268486,0.00016016582],"domain_scores_gemma":[0.9977029,0.00037394182,0.00069711317,0.0003332295,0.00045185382,0.00044105257],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00093094434,0.00031703027,0.0005129158,0.0021979525,0.0010350957,0.0014122981,0.0004060674,0.0005656179,0.00203522],"category_scores_gemma":[0.0015361258,0.00023841963,0.000583296,0.0016652453,0.00028245655,0.0004023195,0.0011529926,0.00061131583,0.0006531638],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00094909134,0.0003052996,0.8829147,0.00010295182,0.00035576097,0.0026447505,0.0005161237,0.0008967787,0.065914266,0.0011563788,0.0054114508,0.03883237],"study_design_scores_gemma":[0.000050810115,0.00015208236,0.9675523,0.000019505678,0.0001295029,0.001301227,0.00020779742,0.0031447397,0.018210923,0.0004423682,0.008751894,0.00003682261],"about_ca_topic_score_codex":0.0055584027,"about_ca_topic_score_gemma":0.011551293,"teacher_disagreement_score":0.0055584027,"about_ca_system_score_codex":0.00039555485,"about_ca_system_score_gemma":0.00038249203,"threshold_uncertainty_score":0.011052072},"labels":[],"label_agreement":null},{"id":"W3096440092","doi":"10.3847/1538-4357/ab3a51","title":"Constraints on Gamma-Ray and Neutrino Emission from NGC 1068 with the MAGIC Telescopes","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Regional Development Fund; Japan Society for the Promotion of Science; Instituto de Astrofísica de Canarias; Institut sur la Nutrition et les Aliments Fonctionnels; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Deutsche Forschungsgemeinschaft; Soochow University; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; National Research Centre; Bundesministerium für Bildung und Forschung; Hrvatska Zaklada za Znanost; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Ministry of Education, Culture, Sports, Science and Technology; Max-Planck-Gesellschaft","keywords":"Neutrino; Galaxy; MAGIC (telescope); Cosmic ray; Neutrino astronomy; Flux (metallurgy); Neutrino detector; Extragalactic background light","score_opus":0.0051477441287865015,"score_gpt":0.1967253834952577,"score_spread":0.1915776393664712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3096440092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958931,0.00015003455,0.0008603887,0.000041445135,0.0000039861325,0.0000040427162,0.00055337645,0.000045950717,0.0024475951],"genre_scores_gemma":[0.9973961,0.0000564841,0.0013897022,0.000013410445,0.0000057142365,0.000006048476,0.0009695969,0.000006125128,0.00015677584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963784,0.00008620086,0.000026793881,0.000096651485,0.0000781919,0.00007428152],"domain_scores_gemma":[0.99851793,0.0006164801,0.00038950072,0.00019140803,0.000119140044,0.0001655396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058976334,0.00043464935,0.00034749336,0.0005586357,0.0002964793,0.0005751246,0.00036326444,0.00037758445,0.0017450502],"category_scores_gemma":[0.0016736161,0.0002332539,0.00030853658,0.00042979003,0.000246621,0.00038701115,0.00047423906,0.00024007476,0.00026695416],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00097036164,0.00006570568,0.9075181,0.000051528932,0.00009281658,0.00038850703,0.00014084655,0.008455658,0.066645,0.001584325,0.00093510764,0.013152008],"study_design_scores_gemma":[0.0000913545,0.00033039378,0.95811236,0.00005802898,0.00009689439,0.00059325015,0.00013472483,0.016440213,0.017895624,0.0013814418,0.0048321183,0.000033518012],"about_ca_topic_score_codex":0.0035602264,"about_ca_topic_score_gemma":0.0062262528,"teacher_disagreement_score":0.0035602264,"about_ca_system_score_codex":0.00043244776,"about_ca_system_score_gemma":0.00017755525,"threshold_uncertainty_score":0.0070790052},"labels":[],"label_agreement":null},{"id":"W3096687606","doi":"10.3847/1538-4357/ac00b2","title":"Collapsar R-process Yields Can Reproduce [Eu/Fe] Abundance Scatter in Metal-poor Stars","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; University of Toronto; National Energy Research Scientific Computing Center; Wissenschaftskolleg zu Berlin; Canadian Institute for Advanced Research; Canada Research Chairs; National Aeronautics and Space Administration; U.S. Department of Energy; Space Telescope Science Institute; National Science Foundation","keywords":"Supernova; Stars; Neutron star; Nucleosynthesis; Population; Abundance (ecology); Yield (engineering)","score_opus":0.01245816151262228,"score_gpt":0.24485351895308152,"score_spread":0.23239535744045925,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3096687606","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913583,0.00004226165,0.0073883934,0.000029569443,0.000002541805,0.000008578143,0.00018599101,0.00009607829,0.0008883337],"genre_scores_gemma":[0.9990029,0.000011558959,0.00067257124,0.00001230724,0.0000014446886,0.000004836561,0.0001239786,0.000028477658,0.000141998],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999696,0.000071740054,0.000020801886,0.00013231547,0.000033773424,0.000045393183],"domain_scores_gemma":[0.9978568,0.000833215,0.0005258829,0.0004518576,0.0001676393,0.00016465623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011276621,0.000621095,0.00053432374,0.00052266626,0.00034734598,0.0011084841,0.0008548766,0.0004750698,0.0011785991],"category_scores_gemma":[0.0037322876,0.0002913431,0.0006066964,0.00034919384,0.00051156356,0.0005812487,0.00080353324,0.00023523763,0.00045547585],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003075943,0.00005040307,0.7310296,0.000052698684,0.0003588247,0.00039768778,0.00027797825,0.2170179,0.03789583,0.0041621337,0.00041984516,0.008029486],"study_design_scores_gemma":[0.000033590757,0.00013934248,0.20467018,0.000012574894,0.000118168784,0.0002970457,0.0001741213,0.77272356,0.014779682,0.005996896,0.0010046349,0.00005025685],"about_ca_topic_score_codex":0.0038987135,"about_ca_topic_score_gemma":0.0021637627,"teacher_disagreement_score":0.0038987135,"about_ca_system_score_codex":0.00058487337,"about_ca_system_score_gemma":0.00023860062,"threshold_uncertainty_score":0.007752061},"labels":[],"label_agreement":null},{"id":"W3096917397","doi":"10.3847/1538-4357/ac59b1","title":"Relativistic Alfvén Waves Entering Charge-starvation in the Magnetospheres of Neutron Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute","funders":"Natural Sciences and Engineering Research Council of Canada; Oak Ridge National Laboratory; Ministry of Colleges and Universities; Flatiron Health; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada; Government of Canada; National Science Foundation","keywords":"Physics; Neutron star; Lorentz factor; Plasma; Magnetosphere; Dissipation; Lorentz force; Magnetic field; Quantum electrodynamics; Kinetic energy; Charge (physics); Astrophysics; Computational physics; Atomic physics; Classical mechanics; Lorentz transformation; Nuclear physics; Quantum mechanics","score_opus":0.013797307137637013,"score_gpt":0.28581184025667805,"score_spread":0.27201453311904106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3096917397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99554056,0.000057376135,0.0022179757,0.00009482957,0.000011537699,0.000008018948,0.000021206892,0.000035052093,0.0020134512],"genre_scores_gemma":[0.99921477,0.000034438137,0.00031275122,0.000015660724,0.0000040108484,0.0000047969156,0.000016423273,0.000011808567,0.00038529327],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999515,0.0000125517645,0.0000024091964,0.0000039722527,0.000010577138,0.000018979857],"domain_scores_gemma":[0.9998276,0.000043002285,0.000048870334,0.000013288713,0.000020249248,0.000046968256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002042717,0.0003857555,0.0003483923,0.0002908444,0.0006235859,0.00082677585,0.00038067647,0.0005518692,0.0007714909],"category_scores_gemma":[0.0007442747,0.0002955057,0.0004975546,0.00019675324,0.0007535072,0.0005086661,0.000636536,0.000374421,0.00013547117],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047891604,0.00020601635,0.027103081,0.00011579769,0.00014058316,0.001298154,0.0006430007,0.88088715,0.058590673,0.023300167,0.00089173275,0.006344849],"study_design_scores_gemma":[0.0001531675,0.00014596886,0.0107128,0.000014370658,0.000023694294,0.00011797213,0.0002554797,0.9772636,0.0045147473,0.006192759,0.00057185924,0.000033515735],"about_ca_topic_score_codex":0.0039392053,"about_ca_topic_score_gemma":0.0019384199,"teacher_disagreement_score":0.0039392053,"about_ca_system_score_codex":0.0008015174,"about_ca_system_score_gemma":0.00041938736,"threshold_uncertainty_score":0.007832587},"labels":[],"label_agreement":null},{"id":"W3097233283","doi":"10.3847/1538-4357/abf6d6","title":"Luminous Type II Short-Plateau Supernovae 2006Y, 2006ai, and 2016egz: A Transitional Class from Stripped Massive Red Supergiants","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Agencia Nacional de Promoción Científica y Tecnológica; Horizon 2020 Framework Programme; Office of Science; New Mexico State University; National Astronomical Observatory of Japan; Nuclear Safety and Security Commission; Consejo Nacional de Investigaciones Científicas y Técnicas; York University; Villum Fonden; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Canadian Institute for Advanced Research; Harvard University; Ohio State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; European Commission; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Japan Society for the Promotion of Science; Council for Higher Education","keywords":"Supernova; Red supergiant; Supergiant; Envelope (radar); Extinction (optical mineralogy); Population; Circumstellar envelope; Type (biology)","score_opus":0.012470513245691395,"score_gpt":0.22565463832203528,"score_spread":0.21318412507634388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3097233283","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981147,0.00006880717,0.0006083378,0.000030410189,0.000004445803,0.000009610189,0.0004013571,0.0000712813,0.00069101906],"genre_scores_gemma":[0.99691147,0.000046951383,0.0009239573,0.000017864892,0.0000057274638,0.0000130920525,0.0018300244,0.000021894994,0.00022902766],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99992335,0.000012314493,0.0000052579476,0.000025526151,0.000010596215,0.000022892036],"domain_scores_gemma":[0.99980074,0.000047346464,0.000028251166,0.00003732602,0.000019976987,0.00006637407],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023106541,0.00043202838,0.0005135111,0.0004972014,0.000378234,0.0009175722,0.0007683841,0.00040947142,0.0018305096],"category_scores_gemma":[0.00063388224,0.00022209233,0.00080013886,0.00036037643,0.00037530996,0.00035718,0.0006678187,0.00044713492,0.00015032727],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068180595,0.00030117895,0.35194445,0.00008752729,0.000381444,0.0003942302,0.00010243444,0.62931824,0.004234538,0.0025811505,0.0014516368,0.008521364],"study_design_scores_gemma":[0.00019052246,0.00020543476,0.14421524,0.000028568138,0.00005794393,0.00020675635,0.00028998533,0.85019594,0.0011474935,0.002069855,0.0013662553,0.000026003674],"about_ca_topic_score_codex":0.009492113,"about_ca_topic_score_gemma":0.011095219,"teacher_disagreement_score":0.009492113,"about_ca_system_score_codex":0.00034075015,"about_ca_system_score_gemma":0.00036480717,"threshold_uncertainty_score":0.018873692},"labels":[],"label_agreement":null},{"id":"W3097342277","doi":"10.3847/1538-4357/abc5bf","title":"The VLA/ALMA Nascent Disk and Multiplicity (VANDAM) Survey of Orion Protostars. IV. Unveiling the Embedded Intermediate-Mass Protostar and Disk within OMC2-FIR3/HOPS-370","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Science and Technology Facilities Council; National Science Foundation","keywords":"Protostar; Physics; Astrophysics; Submillimeter Array; RADIUS; Radiative transfer; Spectral energy distribution; Star formation; Astronomy; Stars; Galaxy; Optics","score_opus":0.016590777235994888,"score_gpt":0.2505682756010169,"score_spread":0.23397749836502202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3097342277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99911636,0.00002750094,0.000040941908,0.000009963486,7.5957365e-7,0.0000031483335,0.00032432887,0.0000069415332,0.00047014497],"genre_scores_gemma":[0.9983967,0.000024518191,0.00030242206,0.000009400823,0.0000029111172,0.00000477842,0.0010023023,0.0000043810287,0.0002526773],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999002,0.00001072844,0.00000449339,0.000027863465,0.000027326987,0.00002931193],"domain_scores_gemma":[0.9997218,0.000018156694,0.00007593109,0.000024925368,0.000034972116,0.00012425965],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001955777,0.00018943018,0.00015116844,0.00070600817,0.0004369658,0.00048356922,0.00023260608,0.0002023811,0.00080342265],"category_scores_gemma":[0.00027735584,0.00011463806,0.0002033366,0.00044554003,0.00017637241,0.00019686791,0.00058187393,0.00014941039,0.00020824297],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013958135,0.00003590668,0.9742863,0.000017818902,0.000029791396,0.00025571138,0.0005058016,0.00024083776,0.019600233,0.00016965118,0.0003322195,0.004386274],"study_design_scores_gemma":[0.0000054787615,0.0000209059,0.99771595,0.0000036570352,0.0000074098098,0.0001008951,0.00023674751,0.00041100237,0.0007211267,0.000026776333,0.000747673,0.0000023960195],"about_ca_topic_score_codex":0.016071342,"about_ca_topic_score_gemma":0.03234601,"teacher_disagreement_score":0.016071342,"about_ca_system_score_codex":0.0005773096,"about_ca_system_score_gemma":0.00025929615,"threshold_uncertainty_score":0.0319556},"labels":[],"label_agreement":null},{"id":"W3097363622","doi":"10.3847/1538-4357/abcf2e","title":"Rise of the Titans: Gas Excitation and Feedback in a Binary Hyperluminous Dusty Starburst Galaxy at z ∼ 6","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Galaxy; Line (geometry); Plateau de Bure Interferometer; Excitation; Star formation; Galaxy merger; Line-of-sight; Binary number","score_opus":0.009622815653105653,"score_gpt":0.21446009880764338,"score_spread":0.20483728315453772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3097363622","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963975,0.000018118964,0.000025664078,0.000013901331,5.8669514e-7,8.174653e-7,0.000019905048,0.000005263273,0.00027597486],"genre_scores_gemma":[0.99981457,0.000005662827,0.000027572014,0.0000055706905,0.0000011355676,4.7952216e-7,0.000029083218,6.952935e-7,0.00011520464],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995947,0.0000037090012,0.0000015784932,0.0000106626,0.000012676566,0.000011940988],"domain_scores_gemma":[0.99985886,0.000012787917,0.000039651837,0.0000063235752,0.000016477203,0.000065838336],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000077574565,0.00010311962,0.00014215424,0.0002786445,0.0003378277,0.0003574152,0.00019101614,0.0001672558,0.00086443604],"category_scores_gemma":[0.00022206546,0.00010586549,0.00007595182,0.000117316136,0.0002029283,0.00013465028,0.00031274726,0.0001721702,0.00014023251],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017515916,0.00007231865,0.90748763,0.000012716713,0.000022469174,0.00069547334,0.00064731314,0.00028984706,0.08520571,0.00021451944,0.00015063892,0.005026228],"study_design_scores_gemma":[0.000002210672,0.00003206404,0.99828774,0.0000011915712,0.000003012877,0.00010973061,0.000099381155,0.0004290086,0.00080977357,0.000031309595,0.00019335945,0.0000012628939],"about_ca_topic_score_codex":0.0072135534,"about_ca_topic_score_gemma":0.01226463,"teacher_disagreement_score":0.0072135534,"about_ca_system_score_codex":0.0004232335,"about_ca_system_score_gemma":0.000091255424,"threshold_uncertainty_score":0.0143431425},"labels":[],"label_agreement":null},{"id":"W3097512588","doi":"10.3847/1538-4357/abb880","title":"The MAVERIC Survey: Radio Catalogs and Source Counts from Deep Very Large Array Imaging of 25 Galactic Globular Clusters","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Australian Research Council; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; David and Lucile Packard Foundation; National Science Foundation","keywords":"Jansky; Globular cluster; Physics; Astrophysics; Milky Way; Spectral index; Pulsar; Astronomy; Millisecond pulsar; Cluster (spacecraft); Radio spectrum; Stars; Galaxy; Spectral line; Radio galaxy","score_opus":0.009557155867741193,"score_gpt":0.20931414927365458,"score_spread":0.19975699340591338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3097512588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97676796,0.0004924181,0.0005462306,0.000047762565,0.000006824998,0.000051224408,0.019975886,0.00020428984,0.0019072713],"genre_scores_gemma":[0.91531557,0.000346087,0.0024433783,0.00005996674,0.000029449504,0.00007179776,0.08049036,0.000084224106,0.0011592811],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994246,0.000069764676,0.000067833964,0.00019210068,0.00015693088,0.000088882334],"domain_scores_gemma":[0.9980287,0.00018275957,0.0005222024,0.00033516675,0.0004624741,0.00046870764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074217323,0.0003238725,0.00026055606,0.0065009245,0.00045855387,0.0008822902,0.0006279258,0.00022876127,0.00200297],"category_scores_gemma":[0.0018182773,0.0001914472,0.00017938013,0.0048611294,0.00020170645,0.00038841643,0.0009786852,0.0001497023,0.00076469703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012297502,0.000046890927,0.96620196,0.000037237114,0.000099159006,0.000108297005,0.0003165882,0.0007536288,0.0028535416,0.00022268496,0.009186229,0.020050839],"study_design_scores_gemma":[0.000015131249,0.000021783286,0.9952722,0.000008073872,0.000016428794,0.00006827213,0.00011382265,0.00040333628,0.0003229698,0.000026781432,0.0037252365,0.0000059599342],"about_ca_topic_score_codex":0.029210666,"about_ca_topic_score_gemma":0.04872755,"teacher_disagreement_score":0.029210666,"about_ca_system_score_codex":0.000559146,"about_ca_system_score_gemma":0.00051687297,"threshold_uncertainty_score":0.05808127},"labels":[],"label_agreement":null},{"id":"W3097772371","doi":"10.3847/1538-4357/abdc21","title":"Two-point Statistics without Bins: A Continuous-function Generalization of the Correlation Function Estimator for Large-scale Structure","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"National Aeronautics and Space Administration","keywords":"Estimator; Basis (linear algebra); Basis function; Mathematics; Function (biology); Cluster analysis; Statistics; Mathematical analysis","score_opus":0.004802046398258959,"score_gpt":0.210870092564974,"score_spread":0.20606804616671504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3097772371","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.014415561,0.00016233228,0.9845351,0.00009628,0.000020457675,0.00001668882,0.000082138045,0.00022817824,0.00044320532],"genre_scores_gemma":[0.47988972,0.00037471033,0.5160296,0.0002757079,0.0002309368,0.00017103343,0.0009052572,0.00038298592,0.0017400705],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.998073,0.0009428917,0.00005886973,0.00029985918,0.00052416004,0.00010118998],"domain_scores_gemma":[0.9836857,0.01025817,0.0013231892,0.002982715,0.0012977214,0.00045248322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00666907,0.00056272844,0.0007941906,0.0017072293,0.00044825985,0.0013965685,0.0018929502,0.0011507664,0.0016157819],"category_scores_gemma":[0.027622778,0.0003702062,0.0007617852,0.0019295334,0.0014786969,0.0019402003,0.0015531295,0.0017980072,0.00056459045],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019765258,0.00016468047,0.030007513,0.00022607847,0.0003133931,0.00034159608,0.00021777571,0.38435194,0.009177922,0.37887713,0.0071971132,0.18892714],"study_design_scores_gemma":[0.000012050504,0.000020384321,0.0032843973,0.000019787256,0.0000123164655,0.000071959905,0.000012872867,0.9509296,0.0011520026,0.042837434,0.0016159486,0.000031359697],"about_ca_topic_score_codex":0.00270247,"about_ca_topic_score_gemma":0.0023233492,"teacher_disagreement_score":0.00666907,"about_ca_system_score_codex":0.000649079,"about_ca_system_score_gemma":0.0010479206,"threshold_uncertainty_score":0.035269856},"labels":[],"label_agreement":null},{"id":"W3098096069","doi":"10.1086/499258","title":"Large Area Mapping at 850 μm. IV. Analysis of the Clump Distribution in the Orion B South Molecular Cloud","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"James Clerk Maxwell Telescope; Physics; Astrophysics; Molecular cloud; Hydrostatic equilibrium; Bolometer; Mass distribution; Orion Nebula; Young stellar object; Telescope; Line (geometry); Astronomy; Galaxy; Star formation; Stars","score_opus":0.007305181982072828,"score_gpt":0.21253521035258313,"score_spread":0.2052300283705103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098096069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9777763,0.0003041225,0.0049537704,0.00032388285,0.0000729247,0.00005387016,0.0047728936,0.00039306175,0.011349051],"genre_scores_gemma":[0.98531693,0.00008514399,0.005126732,0.000060255556,0.000030555202,0.000028308114,0.003024319,0.00006241731,0.0062654326],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999362,0.0000028345503,0.0000020059413,0.000020203375,0.00001925857,0.000019422894],"domain_scores_gemma":[0.9998036,0.000027174272,0.000027705031,0.000020494559,0.00006114929,0.00005998188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015071478,0.00011329033,0.00012420889,0.0009311097,0.0004238314,0.00027478536,0.00026261437,0.00021303701,0.008538407],"category_scores_gemma":[0.00031663003,0.00009315055,0.00019623578,0.00074142043,0.00009765765,0.0001728189,0.000246491,0.00017369264,0.0012503148],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008515442,0.00016291048,0.3328776,0.00021969847,0.00007801523,0.0012982356,0.00063099695,0.0033754404,0.52551734,0.0014629435,0.015382946,0.118142396],"study_design_scores_gemma":[0.00003155698,0.000049214723,0.9774954,0.000014031038,0.000028362781,0.00016100593,0.00017829961,0.0034877737,0.011437923,0.00029811822,0.0068085096,0.000009878208],"about_ca_topic_score_codex":0.007954857,"about_ca_topic_score_gemma":0.015527917,"teacher_disagreement_score":0.008538407,"about_ca_system_score_codex":0.00019652845,"about_ca_system_score_gemma":0.00017813843,"threshold_uncertainty_score":0.028563797},"labels":[],"label_agreement":null},{"id":"W3098130634","doi":"10.1088/0004-637x/809/1/97","title":"HORIZON-SCALE LEPTON ACCELERATION IN JETS: EXPLAINING THE COMPACT RADIO EMISSION IN M87","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Astrophysics; Jet (fluid); Blazar; Radio galaxy; Active galactic nucleus; Astrophysical jet; Black hole (networking); Luminosity; Particle acceleration; Acceleration; Galaxy; Gamma ray; Mechanics; Classical mechanics","score_opus":0.023040433397950293,"score_gpt":0.2562576589781707,"score_spread":0.23321722558022043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098130634","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943018,0.0004479534,0.0030552475,0.0001255342,0.000005832487,0.000007222961,0.000027046883,0.00009685492,0.0019326458],"genre_scores_gemma":[0.99932206,0.000106995656,0.00039994722,0.000018132563,0.000009681996,0.0000022346667,0.000015865431,0.0000071203235,0.00011810247],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996686,0.0000044015783,0.0000021486367,0.0000051864795,0.000008448995,0.0000128989395],"domain_scores_gemma":[0.9998578,0.000044046606,0.000049709506,0.000018947769,0.000009197378,0.000020338539],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017232804,0.0003543975,0.00026903965,0.0005594658,0.0003020185,0.0007779429,0.00061319047,0.0005116333,0.0009873492],"category_scores_gemma":[0.00047837317,0.00018059244,0.00028252983,0.00033383115,0.0007190381,0.0005955086,0.0005683329,0.00026845007,0.00028799704],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086093915,0.00020602644,0.5547582,0.00036901765,0.00013216662,0.016761126,0.003386366,0.04797545,0.25909907,0.063787416,0.0016264193,0.051037904],"study_design_scores_gemma":[0.00020034431,0.0005198902,0.6962265,0.00006712396,0.0001257377,0.0043745073,0.001555654,0.21106313,0.02215467,0.061068054,0.0025879804,0.000056352343],"about_ca_topic_score_codex":0.00085823383,"about_ca_topic_score_gemma":0.0007577571,"teacher_disagreement_score":0.0009873492,"about_ca_system_score_codex":0.00032076184,"about_ca_system_score_gemma":0.000081217026,"threshold_uncertainty_score":0.0033029914},"labels":[],"label_agreement":null},{"id":"W3098153277","doi":"10.3847/1538-4357/abcc72","title":"FIR-luminous [C ii] Emitters in the ALMA-SCUBA-2 COSMOS Survey (AS2COSMOS): The Nature of Submillimeter Galaxies in a 10 Comoving Megaparsec-scale Structure at z ∼ 4.6","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Science Council; National Radio Astronomy Observatory; National Science Foundation","keywords":"Galaxy; Halo; Luminosity; Star formation; Submillimeter Array; Baryon; Accretion (finance); Line (geometry); Emission spectrum","score_opus":0.007941439397213914,"score_gpt":0.2131001048125595,"score_spread":0.20515866541534558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098153277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995672,0.000026718937,0.000028413613,0.000007073456,6.4372955e-7,0.0000012224137,0.000081830694,0.0000060289594,0.00028091707],"genre_scores_gemma":[0.99956137,0.000019848707,0.00008644963,0.0000099205245,0.000004072105,0.000001524576,0.00022380857,0.000001577943,0.00009145097],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999213,0.000009121884,0.0000038703133,0.000022207683,0.000016784754,0.000026678334],"domain_scores_gemma":[0.99956495,0.000042985168,0.00018286136,0.000036451478,0.00004637577,0.00012630934],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018312423,0.00018761451,0.00011982346,0.0010727104,0.0002575655,0.0004542923,0.00019719648,0.00015912585,0.0010740315],"category_scores_gemma":[0.0003545717,0.000114641014,0.00013689908,0.0005454071,0.0001826905,0.00020943151,0.0002893197,0.00013780316,0.00022258714],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051495517,0.000020469342,0.99019134,0.0000047257263,0.00001647312,0.000065754444,0.000113196234,0.000060702478,0.0075211436,0.000059348808,0.00013053072,0.0017647941],"study_design_scores_gemma":[0.0000019563756,0.000010538512,0.99939156,0.0000011090827,0.0000044435205,0.000054103024,0.000034318746,0.000121631194,0.00023813231,0.0000111327545,0.00013025076,8.5904566e-7],"about_ca_topic_score_codex":0.0037676005,"about_ca_topic_score_gemma":0.0055169733,"teacher_disagreement_score":0.0037676005,"about_ca_system_score_codex":0.00015511557,"about_ca_system_score_gemma":0.00008976362,"threshold_uncertainty_score":0.00749135},"labels":[],"label_agreement":null},{"id":"W3098203845","doi":"10.3847/1538-4357/abdb2c","title":"Linear Stability Analysis of a Magnetic Rotating Disk with Ohmic Dissipation and Ambipolar Diffusion","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Ambipolar diffusion; Magnetohydrodynamics; Dimensionless quantity; Instability; Magnetic field; Magnetic diffusivity; Magnetohydrodynamic drive; Thermal diffusivity; Classical mechanics; Mechanics; Plasma; Quantum mechanics","score_opus":0.00814114011921945,"score_gpt":0.23131337152825163,"score_spread":0.22317223140903217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098203845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92281073,0.0005691306,0.0593895,0.00067197613,0.000039812716,0.000060163984,0.00012959023,0.00019448585,0.016134603],"genre_scores_gemma":[0.9942609,0.00009670493,0.0024616169,0.000050759645,0.000029463987,0.000025162426,0.000049035953,0.000030796324,0.0029955704],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998367,0.000044263426,0.0000068985023,0.000027671038,0.00004743006,0.000037035144],"domain_scores_gemma":[0.9992712,0.0002597113,0.00017864731,0.00003922056,0.00017823158,0.00007298617],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036211146,0.0005605144,0.00051931426,0.0008208319,0.000648153,0.0011005208,0.00062254013,0.00067609706,0.0017604622],"category_scores_gemma":[0.0020289188,0.00024957064,0.00049408985,0.00024513027,0.0011893802,0.0006248888,0.0009466192,0.00041157394,0.00030063125],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038073107,0.000084141524,0.009648429,0.00022067262,0.00012885944,0.0009276379,0.00047340422,0.88094187,0.05053278,0.048299786,0.0012473695,0.007114292],"study_design_scores_gemma":[0.000008745419,0.000023037419,0.0005032709,0.000003322484,0.00000490742,0.00001929572,0.000025999174,0.9971981,0.0009070096,0.0011663439,0.00013352651,0.000006449956],"about_ca_topic_score_codex":0.0063525806,"about_ca_topic_score_gemma":0.0015640127,"teacher_disagreement_score":0.0063525806,"about_ca_system_score_codex":0.0009094636,"about_ca_system_score_gemma":0.0005097905,"threshold_uncertainty_score":0.012631178},"labels":[],"label_agreement":null},{"id":"W3098272019","doi":"10.1088/0004-637x/787/1/43","title":"NON-LOCAL THERMODYNAMIC EQUILIBRIUM 1.5D MODELING OF RED GIANT STARS","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Stars; Astrophysics; Observable; Thermodynamic equilibrium; Effective temperature; Spectral line; Radiative equilibrium; Thermodynamics; Astronomy; Radiative transfer; Optics","score_opus":0.011050549926092945,"score_gpt":0.21532841804870043,"score_spread":0.20427786812260748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098272019","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9529787,0.00016660437,0.03506382,0.00022475219,0.000035834983,0.000056825767,0.0019338088,0.00064129155,0.008898482],"genre_scores_gemma":[0.9901901,0.00007320954,0.007554428,0.00005410983,0.00001534838,0.000054419143,0.00089940755,0.00015044621,0.0010086768],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999864,0.000036430334,0.000009457978,0.000041295585,0.000022338461,0.000026607619],"domain_scores_gemma":[0.99973875,0.00006467478,0.00004254184,0.000054166587,0.00004742261,0.000052372834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023637818,0.0004841492,0.00040696704,0.00040890253,0.00035783148,0.00078335294,0.0009270696,0.000788009,0.0013408387],"category_scores_gemma":[0.00079852564,0.00032918566,0.0010644936,0.00036197098,0.00032107238,0.00045560702,0.0005718779,0.00048039455,0.0003611663],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004924758,0.000054199885,0.010705358,0.000027505539,0.000031880765,0.00008372272,0.00009917016,0.9792493,0.004480938,0.0026390026,0.00042825352,0.0021515116],"study_design_scores_gemma":[0.000021397918,0.000012802554,0.0039085695,0.0000025901843,0.0000055845685,0.000026337291,0.000016424483,0.99451196,0.00049954426,0.000523162,0.00046206306,0.0000094664265],"about_ca_topic_score_codex":0.014601186,"about_ca_topic_score_gemma":0.0077699013,"teacher_disagreement_score":0.014601186,"about_ca_system_score_codex":0.0012030242,"about_ca_system_score_gemma":0.0004198918,"threshold_uncertainty_score":0.02903235},"labels":[],"label_agreement":null},{"id":"W3098350763","doi":"10.3847/1538-4357/abd03b","title":"Wave-driven Shocks in Stellar Outbursts: Dynamics, Envelope Heating, and Nascent Blast Waves","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Gordon and Betty Moore Foundation","keywords":"Blast wave; Adiabatic process; Shock wave; Envelope (radar); Shock (circulatory); Waveform; Inflation (cosmology); Differential (mechanical device)","score_opus":0.009560897878977686,"score_gpt":0.22668423621415287,"score_spread":0.2171233383351752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098350763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97867525,0.00008628487,0.01939118,0.000065347376,0.000008656134,0.000008999024,0.000025059086,0.000051660765,0.0016876205],"genre_scores_gemma":[0.99897695,0.000037529673,0.0005839625,0.0000040021387,0.0000031292527,0.0000021191802,0.0000098814035,0.0000067672677,0.0003757072],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99997413,0.0000063418915,0.000002398035,0.0000040523437,0.0000066200187,0.0000064423702],"domain_scores_gemma":[0.99979264,0.00006018957,0.00006420175,0.000019233505,0.000022166803,0.000041543186],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021675663,0.000273471,0.00017913195,0.00023908977,0.00020681944,0.00051462685,0.0002954815,0.00026134102,0.00080568774],"category_scores_gemma":[0.00084825046,0.000119383345,0.00015484041,0.00017669189,0.00046011352,0.0004058627,0.00054909853,0.00032204264,0.00008958198],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030375636,0.00013197116,0.114737436,0.00012421758,0.000049089966,0.001338567,0.00077938475,0.706403,0.101170816,0.05187961,0.0004486521,0.022633366],"study_design_scores_gemma":[0.000019584415,0.000050723123,0.023569765,0.000009127868,0.000005558085,0.00011364393,0.00010481538,0.96352214,0.005692451,0.0066766366,0.00022464577,0.000010858794],"about_ca_topic_score_codex":0.0013758314,"about_ca_topic_score_gemma":0.00079556386,"teacher_disagreement_score":0.0013758314,"about_ca_system_score_codex":0.00023274962,"about_ca_system_score_gemma":0.00012384652,"threshold_uncertainty_score":0.0027356744},"labels":[],"label_agreement":null},{"id":"W3098636927","doi":"10.3847/1538-4357/abca3a","title":"Correlated X-Ray and Optical Variability in the O-type Supergiant ζ Puppis","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec","funders":"","keywords":"Supergiant; Light curve; Rotation period; Wavelength; Stellar rotation; Stars; Starspot; Variable star; Maxima; Phase (matter)","score_opus":0.009271277162610432,"score_gpt":0.21926836941055314,"score_spread":0.20999709224794272,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098636927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994898,0.000018257062,0.000036027843,0.000007065196,8.197064e-7,0.00000148195,0.000077249075,0.0000033591937,0.0003659361],"genre_scores_gemma":[0.99958366,0.000024101473,0.00006034118,0.0000054356433,0.0000028194102,0.0000018707724,0.0001900193,0.0000025909376,0.0001291124],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994254,0.0000056358413,0.000002762749,0.000018558174,0.000017058772,0.000013455945],"domain_scores_gemma":[0.9998148,0.000019359826,0.00006561254,0.000018585308,0.000025821952,0.00005580122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015100492,0.00015247524,0.00016106716,0.0007504205,0.00036061,0.0004121511,0.00017304132,0.00011160753,0.00075348094],"category_scores_gemma":[0.00039304805,0.00010575712,0.00011418639,0.00032311966,0.0003007316,0.00016353875,0.00044801162,0.00016737865,0.0002179975],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019819435,0.00004331587,0.9415908,0.000023286273,0.000044698452,0.0007897153,0.0003438716,0.00032296305,0.04948501,0.0002021485,0.00022920257,0.00672672],"study_design_scores_gemma":[0.0000015525403,0.000021736783,0.9990125,0.0000015014236,0.0000025728975,0.00011870467,0.000076589335,0.00015897975,0.0003621923,0.000027816754,0.00021483266,0.0000010729291],"about_ca_topic_score_codex":0.002857743,"about_ca_topic_score_gemma":0.0035016646,"teacher_disagreement_score":0.002857743,"about_ca_system_score_codex":0.00024830372,"about_ca_system_score_gemma":0.00009010133,"threshold_uncertainty_score":0.00568223},"labels":[],"label_agreement":null},{"id":"W3098658987","doi":"10.1088/0004-637x/748/2/79","title":"PLANETESIMAL AND PROTOPLANET DYNAMICS IN A TURBULENT PROTOPLANETARY DISK: IDEAL STRATIFIED DISKS","year":2012,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Protoplanet; Physics; Planetesimal; Protoplanetary disk; Turbulence; Astrophysics; Planet; Classical mechanics; Mechanics","score_opus":0.010076489029096771,"score_gpt":0.2337874271100889,"score_spread":0.22371093808099213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098658987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968225,0.00007908838,0.002150287,0.00003999756,0.000005754183,0.000010228068,0.000075321776,0.000020273084,0.0007966737],"genre_scores_gemma":[0.9986815,0.0000649625,0.0009986314,0.000013502682,0.0000033300043,0.000011099326,0.000049276478,0.00000626194,0.0001714419],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999254,0.00002075525,0.000005864077,0.000013633268,0.000012933054,0.000021460071],"domain_scores_gemma":[0.9997247,0.00007444513,0.000075861615,0.00003978245,0.000027158863,0.000058018082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020291303,0.00039896904,0.00041038997,0.0002528259,0.00033744916,0.00072826626,0.0005683061,0.0004586586,0.00039408845],"category_scores_gemma":[0.0009035837,0.00017656256,0.0003961981,0.00020396982,0.00089015847,0.00045365165,0.0006566472,0.00028078113,0.00007028389],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049685396,0.00017239492,0.023263397,0.000074747906,0.000079838566,0.00036273236,0.00024603834,0.9466629,0.01992445,0.0070756064,0.00013802145,0.0015030401],"study_design_scores_gemma":[0.000095704505,0.00011973645,0.006836113,0.000008986487,0.000026272422,0.000051340205,0.00009246331,0.98973686,0.0016710951,0.0012023278,0.00014478511,0.000014417367],"about_ca_topic_score_codex":0.008878788,"about_ca_topic_score_gemma":0.0026688944,"teacher_disagreement_score":0.008878788,"about_ca_system_score_codex":0.0005622708,"about_ca_system_score_gemma":0.00037370156,"threshold_uncertainty_score":0.01765424},"labels":[],"label_agreement":null},{"id":"W3098665185","doi":"10.3847/1538-4357/abc881","title":"New Horizons Observations of the Cosmic Optical Background","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":79,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"COSMIC cancer database; Astronomy; New horizons; Physics; Cosmic microwave background; Astrophysics; Optics","score_opus":0.027899490786487503,"score_gpt":0.2422279675063888,"score_spread":0.2143284767199013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098665185","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98119146,0.00035414414,0.0019104225,0.00007333688,0.000019883642,0.00001712285,0.00319151,0.00020650584,0.01303548],"genre_scores_gemma":[0.9934788,0.00012283745,0.0019410026,0.000020247053,0.00003336469,0.000007875737,0.0030211785,0.000030777348,0.0013438504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969137,0.000019814253,0.000008166586,0.00007548743,0.00014106417,0.00006406913],"domain_scores_gemma":[0.9989631,0.00006937798,0.0003447104,0.00011727979,0.00018674746,0.00031871078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045971898,0.0002252391,0.00017737757,0.0012581378,0.00024602353,0.00044786456,0.00027322109,0.00008113799,0.0022615218],"category_scores_gemma":[0.00094695884,0.00011148117,0.00017225363,0.00065126293,0.00014380034,0.00038416698,0.00066314975,0.00036108092,0.00025536993],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006109724,0.00011591495,0.7928337,0.00015041736,0.00021392365,0.0005479647,0.0015785726,0.0030859385,0.05006363,0.00444057,0.007924771,0.13843365],"study_design_scores_gemma":[0.00001179824,0.000052883304,0.98615855,0.000017092696,0.00001882802,0.00010609873,0.000098714445,0.001464041,0.0025558432,0.0005230322,0.008978106,0.000015022935],"about_ca_topic_score_codex":0.015998926,"about_ca_topic_score_gemma":0.031213528,"teacher_disagreement_score":0.015998926,"about_ca_system_score_codex":0.0008555451,"about_ca_system_score_gemma":0.00015355156,"threshold_uncertainty_score":0.031811595},"labels":[],"label_agreement":null},{"id":"W3098896129","doi":"10.3847/0004-637x/817/2/107","title":"ATMOSPHERES OF LOW-MASS PLANETS: THE “BOIL-OFF”","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":229,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Planet; Photoevaporation; Physics; Astrophysics; Planetary mass; RADIUS; Gas giant; Astronomy; Atmosphere (unit); Exoplanet; Protoplanetary disk; Meteorology","score_opus":0.007370412100678313,"score_gpt":0.20721900113462488,"score_spread":0.19984858903394656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3098896129","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9904687,0.00090879883,0.0027766575,0.00055207603,0.000037427384,0.0000079200645,0.00006439295,0.000084829364,0.005099166],"genre_scores_gemma":[0.9993734,0.000070574744,0.0001967039,0.000037542384,0.000007077549,0.0000018006326,0.000036806316,0.000010746681,0.00026547897],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999261,0.000009074103,0.0000020097123,0.000017674738,0.000014797457,0.000030329707],"domain_scores_gemma":[0.999803,0.000033476874,0.000052645075,0.000023321998,0.000020872612,0.000066632485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106954656,0.00020037174,0.00023686753,0.00028944248,0.0008676015,0.00087566546,0.0005769004,0.00059549895,0.0021700582],"category_scores_gemma":[0.00046603885,0.00017008782,0.00017159658,0.00012466323,0.0009021956,0.0008480448,0.0012240969,0.0009727371,0.00048375037],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065374403,0.00028782204,0.31013203,0.00041501631,0.00012567552,0.0066679604,0.004826975,0.0069197225,0.60812205,0.028818792,0.0062646857,0.02676549],"study_design_scores_gemma":[0.00011832427,0.00064164394,0.6805285,0.00014950117,0.00015737671,0.00840809,0.0047967057,0.098671,0.13120331,0.02262577,0.052507557,0.00019226172],"about_ca_topic_score_codex":0.0020500391,"about_ca_topic_score_gemma":0.0010005764,"teacher_disagreement_score":0.0021700582,"about_ca_system_score_codex":0.00050883216,"about_ca_system_score_gemma":0.000090058726,"threshold_uncertainty_score":0.0072595477},"labels":[],"label_agreement":null},{"id":"W3099187547","doi":"10.3847/1538-4357/ab44a0","title":"Preprocessing among the Infalling Galaxy Population of EDisCS Clusters","year":2019,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Galaxy; Redshift; Galaxy cluster; Cluster (spacecraft); Population; Sigma; RADIUS; Virial theorem; Coma Cluster; Astronomy","score_opus":0.0057663897716677395,"score_gpt":0.21129748085906003,"score_spread":0.2055310910873923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3099187547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918646,0.000035443405,0.00007024389,0.000022473576,0.0000011554619,0.000003865386,0.0002855016,0.000010504573,0.00038427545],"genre_scores_gemma":[0.99807954,0.00002582672,0.00014471037,0.000019668121,0.000003007874,0.00000287688,0.0013962126,0.000005250324,0.00032288837],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995684,0.000037241654,0.000033646058,0.00012843256,0.00008663752,0.00014570981],"domain_scores_gemma":[0.9984074,0.00019311467,0.00042467544,0.00024050199,0.00030542488,0.00042888388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035576374,0.00021551354,0.00034965453,0.001254463,0.000740771,0.0010765259,0.0007058901,0.00024177227,0.0013452165],"category_scores_gemma":[0.0023389494,0.0001863096,0.00025878195,0.0011060007,0.00056661264,0.00048769248,0.0011321633,0.00028155692,0.0002886912],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010851259,0.000020685731,0.99565375,0.000005997674,0.00001508704,0.00006476055,0.00029428306,0.00013778321,0.0014312657,0.00010351085,0.00014788283,0.0020165332],"study_design_scores_gemma":[0.0000012393182,0.0000092916525,0.9990613,0.0000014302851,0.0000042395777,0.00003821272,0.00017500589,0.00020723387,0.0002923818,0.000023778168,0.00018374827,0.0000022454212],"about_ca_topic_score_codex":0.025605913,"about_ca_topic_score_gemma":0.024785439,"teacher_disagreement_score":0.025605913,"about_ca_system_score_codex":0.00075947586,"about_ca_system_score_gemma":0.0005254591,"threshold_uncertainty_score":0.05091375},"labels":[],"label_agreement":null},{"id":"W3099446145","doi":"10.3847/1538-4357/abcc6c","title":"JCMT POL-2 and BISTRO Survey Observations of Magnetic Fields in the L1689 Molecular Cloud","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"National Key Research and Development Program of China; Japan Society for the Promotion of Science; National Research Foundation of Korea; Science and Technology Facilities Council; Chinese Academy of Sciences; National Natural Science Foundation of China","keywords":"James Clerk Maxwell Telescope; Ophiuchus; Molecular cloud; Magnetic field; Protostar; Spitzer Space Telescope; Polarization (electrochemistry); Star formation; Protein filament","score_opus":0.02131537614387939,"score_gpt":0.24678686736564517,"score_spread":0.2254714912217658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3099446145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977034,0.00004899796,0.000115836956,0.00003355792,0.0000042580173,0.000008024813,0.0009942852,0.000036938614,0.0010546955],"genre_scores_gemma":[0.99739504,0.000040730512,0.0005108561,0.000030786814,0.00001780756,0.000009365812,0.0016928221,0.0000104707115,0.00029217656],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987257,0.000008334792,0.000005979636,0.000035739784,0.000047292913,0.000030060633],"domain_scores_gemma":[0.9995732,0.000017392917,0.00015180682,0.000028734925,0.00007216,0.00015669636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013389808,0.00021946823,0.0001908268,0.0011213762,0.00039597438,0.00031440228,0.00029775797,0.00020960653,0.0010964455],"category_scores_gemma":[0.00035735386,0.00013735621,0.00010717794,0.00056683517,0.00015639116,0.00022900746,0.0005469598,0.00020801832,0.00035516373],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033849094,0.0001042103,0.89457214,0.00004451461,0.00005958992,0.0004995476,0.00037172574,0.0005290087,0.08735969,0.0001437122,0.0018870438,0.014090224],"study_design_scores_gemma":[0.00001330366,0.00002544952,0.99668103,0.0000050177687,0.000008633022,0.00010210445,0.000073734795,0.0005554672,0.0013481145,0.000016853832,0.0011661841,0.000004109119],"about_ca_topic_score_codex":0.011806115,"about_ca_topic_score_gemma":0.030609159,"teacher_disagreement_score":0.011806115,"about_ca_system_score_codex":0.0004374526,"about_ca_system_score_gemma":0.00020568866,"threshold_uncertainty_score":0.023474753},"labels":[],"label_agreement":null},{"id":"W3100333340","doi":"10.1086/523096","title":"Looking for Super‐Earths in the HD 189733 System: A Search for Transits in<i>MOST</i>Space‐based Photometry","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory; Université de Montréal; Saint Mary's University; University of Toronto; St. Mary's University; University of British Columbia","funders":"","keywords":"Exoplanet; Physics; Planet; Photometry (optics); Astronomy; Stars; Astrophysics; Hot Jupiter; Transit (satellite)","score_opus":0.018833630728097017,"score_gpt":0.2684553938150074,"score_spread":0.24962176308691036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3100333340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988722,0.000027712318,0.00024471257,0.000014211144,9.3939644e-7,0.0000029910923,0.00044390268,0.00001576023,0.0003774407],"genre_scores_gemma":[0.9985567,0.000021306285,0.0005027061,0.000013721283,0.0000024256904,0.0000023423183,0.0008201401,0.0000058309834,0.00007484543],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999144,0.000011140947,0.0000043169866,0.00002477592,0.000018206681,0.000027186668],"domain_scores_gemma":[0.99967134,0.000054433447,0.00012133061,0.00003968295,0.000029490791,0.000083749226],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016153888,0.000121824196,0.00024537885,0.0004938704,0.0006486956,0.00035882316,0.00013887072,0.00015228635,0.0010064322],"category_scores_gemma":[0.0003017296,0.000090062764,0.00021541926,0.0007481125,0.00019759135,0.00019573777,0.00024689626,0.0002205885,0.00018268511],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053784135,0.00008285164,0.9294294,0.000042440835,0.000077509554,0.0005314658,0.0004039178,0.0012211386,0.05105501,0.00045501487,0.0006957921,0.015467518],"study_design_scores_gemma":[0.00000803218,0.00004896191,0.9951407,0.000002063895,0.000020127778,0.0002686162,0.00009932195,0.0006539742,0.0027664115,0.00007288287,0.000913268,0.000005693534],"about_ca_topic_score_codex":0.010999624,"about_ca_topic_score_gemma":0.027081594,"teacher_disagreement_score":0.010999624,"about_ca_system_score_codex":0.00036395993,"about_ca_system_score_gemma":0.0002505981,"threshold_uncertainty_score":0.02187121},"labels":[],"label_agreement":null},{"id":"W3101411268","doi":"10.3847/1538-4357/abca99","title":"The JCMT BISTRO Survey: Alignment between Outflows and Magnetic Fields in Dense Cores/Clumps","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council","keywords":"Physics; Magnetic field; Astrophysics; Protostar; Star formation; Outflow; Magnetohydrodynamics; Turbulence; Eddy current brake; Magnetic energy; Observable; Stars; Mechanics","score_opus":0.015730759246346662,"score_gpt":0.24662764002961354,"score_spread":0.23089688078326687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3101411268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997207,0.00007146275,0.00011414239,0.000014516116,0.0000028358918,0.000005818639,0.001789304,0.000029866545,0.000765035],"genre_scores_gemma":[0.99521554,0.000049566508,0.00031154283,0.000017435308,0.000016794065,0.0000067598908,0.0042040325,0.000015541546,0.00016276025],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997192,0.00003142421,0.000026105829,0.000078775214,0.00008457022,0.000059841983],"domain_scores_gemma":[0.9980646,0.00013927273,0.001020045,0.0001913421,0.0002508966,0.00033389055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003015642,0.00019615664,0.00023488264,0.002332911,0.00028391072,0.00056149723,0.0002633209,0.00022026629,0.0010690042],"category_scores_gemma":[0.0011858784,0.00012439118,0.00016355794,0.0016648608,0.00023978378,0.00027654573,0.0007188685,0.00013901327,0.00036772783],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010697573,0.000017389122,0.98872256,0.00002325994,0.000034098754,0.00007900107,0.00015261874,0.00013647867,0.006762167,0.000038914306,0.00050144683,0.003425147],"study_design_scores_gemma":[0.000002540406,0.000007739001,0.9992581,0.0000020780017,0.0000047415747,0.000033728862,0.00003577349,0.00018020552,0.0002235696,0.0000038068715,0.00024650703,0.0000012254435],"about_ca_topic_score_codex":0.009270965,"about_ca_topic_score_gemma":0.015157085,"teacher_disagreement_score":0.009270965,"about_ca_system_score_codex":0.0002936742,"about_ca_system_score_gemma":0.00022032742,"threshold_uncertainty_score":0.018433988},"labels":[],"label_agreement":null},{"id":"W3101772101","doi":"10.3847/1538-4357/abec84","title":"Outflows from Super Star Clusters in the Central Starburst of NGC 253","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Millimeter; Galaxy; Outflow; Star formation; Redshift; Stars; Submillimeter Array; Interstellar medium; Astronomy; Cluster (spacecraft); Star cluster","score_opus":0.01055668669098868,"score_gpt":0.22659987554445066,"score_spread":0.21604318885346196,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3101772101","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997309,0.000009993145,0.00004263711,0.0000040930745,6.6604355e-7,7.3890203e-7,0.000043951983,0.000007954445,0.00015902793],"genre_scores_gemma":[0.9997429,0.000009420782,0.000046720816,0.0000029166388,0.0000012110612,7.9280153e-7,0.00012270571,0.0000013142096,0.000071992356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995697,0.0000038194653,0.0000033405145,0.00001420891,0.000008799322,0.000012802937],"domain_scores_gemma":[0.99975187,0.000043602584,0.000081944374,0.000016772085,0.000023762586,0.00008208132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109258355,0.00017835853,0.00020377855,0.00028544635,0.00028114437,0.0003671693,0.00017646175,0.00016123263,0.00087428605],"category_scores_gemma":[0.00026132606,0.000113552385,0.00013377365,0.00024708748,0.00017797714,0.00011743298,0.00024858845,0.0001244669,0.000120831435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037869945,0.00007475811,0.9412141,0.000026417734,0.00005145385,0.0013257164,0.00038787068,0.0047711004,0.046679564,0.00027408355,0.00033167194,0.004484649],"study_design_scores_gemma":[0.0000120130835,0.000045498637,0.9936738,0.0000032219134,0.000011708888,0.00016624214,0.00012925954,0.004578352,0.0010944403,0.000080693004,0.00020074596,0.000003982556],"about_ca_topic_score_codex":0.0123968255,"about_ca_topic_score_gemma":0.013737273,"teacher_disagreement_score":0.0123968255,"about_ca_system_score_codex":0.00038703866,"about_ca_system_score_gemma":0.00013422788,"threshold_uncertainty_score":0.024649322},"labels":[],"label_agreement":null},{"id":"W3102103354","doi":"10.1086/323437","title":"Ultraviolet Broad Absorption Features and the Spectral Energy Distribution of the Quasar PG 1351+64","year":2001,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"QSOS; Astrophysics; Quasar; Redshift; Physics; Lyman limit; Galaxy; Opacity; Emission spectrum; Spectral line; Absorption spectroscopy; Ultraviolet; Astronomy; Spectral energy distribution; Optics; Intergalactic medium","score_opus":0.006340577425442262,"score_gpt":0.20965424161970453,"score_spread":0.20331366419426228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102103354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984238,0.00011168364,0.000101948084,0.000018432784,0.0000011363264,0.0000017798433,0.00034792884,0.000024118663,0.0009691119],"genre_scores_gemma":[0.9992136,0.00004664952,0.00010986065,0.0000070670367,0.000003057712,0.0000014668643,0.0004545382,0.000003174609,0.0001606062],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999658,0.0000015355741,0.0000013757475,0.000010730269,0.000008091943,0.000012378493],"domain_scores_gemma":[0.99987984,0.000010886529,0.000058164715,0.000005164578,0.000008979011,0.000036946505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004650747,0.00018375916,0.00011334446,0.0008047029,0.00017430169,0.00034313116,0.00014482233,0.0001302824,0.0017399811],"category_scores_gemma":[0.00015964638,0.00007481219,0.000106458196,0.0006580659,0.00013820927,0.00012925979,0.00023527598,0.00018297152,0.0002165294],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038386745,0.00012100006,0.79494834,0.00010271356,0.000078663135,0.0008664974,0.00034189707,0.0027022052,0.16803038,0.0006246982,0.0010127744,0.030786986],"study_design_scores_gemma":[0.0000030946899,0.000021548462,0.9982799,0.0000024180115,0.000007883915,0.00015399174,0.000031821968,0.000409499,0.0006499695,0.00004375659,0.00039308023,0.000003091413],"about_ca_topic_score_codex":0.005951673,"about_ca_topic_score_gemma":0.006236455,"teacher_disagreement_score":0.005951673,"about_ca_system_score_codex":0.0003325897,"about_ca_system_score_gemma":0.00006277069,"threshold_uncertainty_score":0.011834085},"labels":[],"label_agreement":null},{"id":"W3102292951","doi":"10.3847/1538-4357/abc341","title":"Quasars That Have Transitioned from Radio-quiet to Radio-loud on Decadal Timescales Revealed by VLASS and FIRST","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Quasar; Astrophysics; Physics; Active galactic nucleus; Sky; Redshift; QUIET; Population; Astronomy; Cosmic microwave background; Galaxy; Demography","score_opus":0.011264956136627523,"score_gpt":0.20881970727832158,"score_spread":0.19755475114169405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102292951","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989827,0.00018610006,0.00015582806,0.000036576806,0.0000060591556,0.0000017862044,0.0002533221,0.000008099028,0.00036943096],"genre_scores_gemma":[0.99962723,0.000039642277,0.000042219956,0.0000108699105,0.0000065233617,0.0000012991978,0.00016479052,0.0000010404611,0.00010635455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991524,0.000010789549,0.000007364685,0.000024351475,0.000016810669,0.000025435622],"domain_scores_gemma":[0.99921215,0.000071348375,0.0004033935,0.000061910614,0.000089477086,0.00016167139],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026125656,0.00009814254,0.00013410546,0.0008334578,0.00021076665,0.00050118595,0.00013712014,0.00014403842,0.0011313338],"category_scores_gemma":[0.00067923125,0.000067906105,0.00011371275,0.0005092774,0.0002030917,0.00036473922,0.00038883762,0.00030646156,0.0002022453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045937486,0.000017416207,0.98954153,0.000008863963,0.000027649541,0.000091128655,0.0002011057,0.00005830971,0.004622401,0.00007692531,0.000108037704,0.005200611],"study_design_scores_gemma":[3.356124e-7,0.000011512215,0.9995041,0.0000011923007,0.0000037861219,0.00006575122,0.000055683955,0.0000319699,0.00013612543,0.000018854038,0.00016965398,0.0000010596676],"about_ca_topic_score_codex":0.0013901733,"about_ca_topic_score_gemma":0.0025458387,"teacher_disagreement_score":0.0013901733,"about_ca_system_score_codex":0.00016589652,"about_ca_system_score_gemma":0.000049247064,"threshold_uncertainty_score":0.0037846565},"labels":[],"label_agreement":null},{"id":"W3102443279","doi":"10.1088/0004-637x/809/2/173","title":"AN EXTREME STARBURST IN THE CORE OF A RICH GALAXY CLUSTER AT<i>z</i>= 1.7","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Dalhousie University; University of Toronto; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Space Telescope Science Institute; Office of Science; National Aeronautics and Space Administration; California Institute of Technology; High Energy Physics; W. M. Keck Foundation; U.S. Department of Energy","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Star formation; Luminosity; Galaxy cluster; Spitzer Space Telescope; Redshift; Type-cD galaxy; Brightest cluster galaxy; Telescope","score_opus":0.02723480884089547,"score_gpt":0.24280338818569194,"score_spread":0.21556857934479648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102443279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994999,0.0000266557,0.000059507973,0.000018745652,0.000002041978,0.0000024578112,0.00006410111,0.00001248245,0.0003142186],"genre_scores_gemma":[0.99916553,0.00002068715,0.00022129473,0.000028643963,0.0000065616127,0.000001832959,0.00035064018,0.0000035811695,0.00020114882],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999038,0.0000069341763,0.000003642996,0.000024061415,0.00002187948,0.000039589875],"domain_scores_gemma":[0.9996728,0.000018061372,0.0000852415,0.000027354976,0.000040010113,0.00015655467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017723945,0.00013718265,0.00024206845,0.00030896396,0.00054950535,0.0004515021,0.00023730741,0.00016928883,0.0007251329],"category_scores_gemma":[0.00028416226,0.00011233186,0.00013868148,0.00024935658,0.00026028545,0.00014544619,0.00046853485,0.000236451,0.00025110322],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033814576,0.00011400698,0.9367538,0.000021385393,0.00006083504,0.00114461,0.0005907876,0.0002993866,0.054518547,0.00023534516,0.0007839304,0.005139271],"study_design_scores_gemma":[0.000005512668,0.00006363953,0.99771535,0.0000020143887,0.000012281489,0.00034946523,0.00008130721,0.00024816804,0.0010318855,0.000044487842,0.0004422418,0.0000036252845],"about_ca_topic_score_codex":0.0049560308,"about_ca_topic_score_gemma":0.008064985,"teacher_disagreement_score":0.0049560308,"about_ca_system_score_codex":0.00029097087,"about_ca_system_score_gemma":0.00015068088,"threshold_uncertainty_score":0.009854376},"labels":[],"label_agreement":null},{"id":"W3102796505","doi":"10.3847/1538-4357/abc7cb","title":"The Herschel Orion Protostar Survey: Far-infrared Photometry and Colors of Protostars and Their Variations across Orion A and B*","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Star formation; Photometry (optics); Flux (metallurgy); Molecular cloud; Stars; Orion Nebula","score_opus":0.017003628615900906,"score_gpt":0.2605163798416832,"score_spread":0.24351275122578228,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102796505","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747485,0.00014334937,0.000067544795,0.000022232081,0.0000013898483,0.000002988512,0.0013889793,0.000011693203,0.0008869875],"genre_scores_gemma":[0.9975413,0.000082259125,0.00022059646,0.000018945055,0.000004717084,0.0000044438166,0.0018416484,0.000008458923,0.0002775015],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997142,0.00004105957,0.000021000276,0.00010264291,0.00007004025,0.00005106872],"domain_scores_gemma":[0.9990864,0.00012672583,0.00035212535,0.000102801445,0.00012514007,0.00020669667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037348698,0.0001512424,0.0001976411,0.0015966258,0.00030524706,0.0005314816,0.00021066058,0.00028186123,0.0011841909],"category_scores_gemma":[0.0007027736,0.00011798961,0.00014886417,0.0010145071,0.0002726509,0.00040897835,0.0005552396,0.00015468575,0.0004004723],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048996924,0.000012941382,0.9924137,0.00000904637,0.000031360603,0.000025218185,0.00013987854,0.00008819034,0.00413105,0.000051626797,0.00021037142,0.0028377373],"study_design_scores_gemma":[7.21991e-7,0.0000029577077,0.99975723,8.053562e-7,0.0000012061361,0.000013374419,0.000030068433,0.000031782896,0.000048086942,0.0000049470395,0.0001082999,5.178659e-7],"about_ca_topic_score_codex":0.011817201,"about_ca_topic_score_gemma":0.024495386,"teacher_disagreement_score":0.011817201,"about_ca_system_score_codex":0.00032510527,"about_ca_system_score_gemma":0.00013628225,"threshold_uncertainty_score":0.023496807},"labels":[],"label_agreement":null},{"id":"W3102804486","doi":"10.1088/0004-637x/694/1/l6","title":"VERY-LONG-BASELINE INTERFEROMETRY OBSERVATIONS OF SN 2008D","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Very-long-baseline interferometry; Physics; Astrophysics; Proper motion; Epoch (astronomy); Supernova; Jet (fluid); Line-of-sight; Flux (metallurgy); Interferometry; Outflow; Position (finance); Centroid; Very Long Baseline Array; Limit (mathematics); Astrophysical jet; Astronomy; Quasar; Galaxy; Active galactic nucleus; Geometry; Mechanics; Stars; Meteorology","score_opus":0.018653317191959888,"score_gpt":0.2471127775262563,"score_spread":0.2284594603342964,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102804486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99541605,0.00015648206,0.0010249144,0.00007344554,0.000015626038,0.000019732508,0.0015907899,0.00006645415,0.0016364232],"genre_scores_gemma":[0.98645186,0.00011481014,0.0060484544,0.00015385874,0.000037948856,0.00005643083,0.0065023783,0.00001805336,0.0006161597],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999811,0.000020361535,0.000012034026,0.00005348112,0.000059088103,0.000044084256],"domain_scores_gemma":[0.9995166,0.000035603116,0.00015496233,0.000052976495,0.000097768476,0.00014203797],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042879075,0.00026269327,0.00027405514,0.000993511,0.00044862277,0.0003648157,0.00042112623,0.00037991733,0.00031903625],"category_scores_gemma":[0.00054506614,0.00026987048,0.00023874169,0.000493569,0.00020334533,0.00024837875,0.0007096812,0.00051543344,0.00024550286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005656074,0.00038336826,0.8367013,0.00007708618,0.00014737564,0.0007311857,0.00046112644,0.0006162473,0.13261516,0.000433107,0.002448223,0.024820272],"study_design_scores_gemma":[0.000022257245,0.00008735989,0.9952193,0.000005183749,0.000017606677,0.0003353644,0.000044835542,0.00059019605,0.0016236323,0.000062885716,0.0019822083,0.000009152204],"about_ca_topic_score_codex":0.0040291967,"about_ca_topic_score_gemma":0.016399687,"teacher_disagreement_score":0.0040291967,"about_ca_system_score_codex":0.00051585486,"about_ca_system_score_gemma":0.0002868675,"threshold_uncertainty_score":0.00801146},"labels":[],"label_agreement":null},{"id":"W3102849512","doi":"10.3847/1538-4357/abc7c4","title":"The Rapid Buildup of Massive Early-type Galaxies: Supersolar Metallicity, High Velocity Dispersion, and Young Age for an Early-type Galaxy at z = 3.35","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":46,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Star formation; Galaxy; Metallicity; Stellar population; Stellar mass; Velocity dispersion; Redshift; Population","score_opus":0.013755637664756518,"score_gpt":0.21955877695270912,"score_spread":0.2058031392879526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102849512","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991109,0.00008573356,0.0001532685,0.000015509566,0.0000015673174,0.00000223607,0.00011164193,0.00001607111,0.0005030844],"genre_scores_gemma":[0.9996043,0.000019065064,0.000117186086,0.0000074734808,0.000002312848,8.082011e-7,0.00011640617,0.0000019946933,0.00013065399],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999324,0.000004080009,0.0000027299668,0.000021904221,0.000013989345,0.000024945935],"domain_scores_gemma":[0.99960035,0.000032170254,0.0001458051,0.000033155695,0.000060128375,0.00012831719],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001942113,0.00018710626,0.00014639359,0.00066586735,0.00025228725,0.00054456503,0.0002074469,0.00026603998,0.00061227445],"category_scores_gemma":[0.00035735863,0.00011018272,0.00013415495,0.0003460312,0.00023805685,0.00024343748,0.00026150304,0.0002569165,0.00019175558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008967461,0.000027174061,0.9552846,0.000013056111,0.00002001478,0.0001536658,0.00031737186,0.00012522451,0.03957985,0.00027160885,0.00012709574,0.0039907186],"study_design_scores_gemma":[6.3003046e-7,0.000010120308,0.9988207,8.2497485e-7,0.0000024840815,0.00006005043,0.000025305055,0.00008065578,0.00085006683,0.000026076572,0.00012194942,0.00000110628],"about_ca_topic_score_codex":0.0042484505,"about_ca_topic_score_gemma":0.0063103056,"teacher_disagreement_score":0.0042484505,"about_ca_system_score_codex":0.00037158767,"about_ca_system_score_gemma":0.00009333354,"threshold_uncertainty_score":0.008447409},"labels":[],"label_agreement":null},{"id":"W3102882083","doi":"10.3847/0004-637x/820/1/28","title":"THE DENSE MATTER EQUATION OF STATE FROM NEUTRON STAR RADIUS AND MASS MEASUREMENTS","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":405,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Physics; Equation of state; RADIUS; Astrophysics; Context (archaeology); Neutron; Thermonuclear fusion; Saturation (graph theory); Nuclear physics; Computational physics; Quantum mechanics; Plasma","score_opus":0.023118571205503882,"score_gpt":0.289232155963476,"score_spread":0.26611358475797214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3102882083","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97328305,0.0005720787,0.021058373,0.000046669862,0.000006089565,0.000018252073,0.0012953636,0.000107891756,0.0036122794],"genre_scores_gemma":[0.9933629,0.00018358468,0.0049897064,0.000008570621,0.0000065758873,0.000008990307,0.0011694849,0.000021850521,0.00024835905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994678,0.00010804699,0.00005083027,0.00013965514,0.00020426096,0.000029445473],"domain_scores_gemma":[0.9978204,0.0007734968,0.00071727287,0.00032330604,0.0002950247,0.00007058123],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011964138,0.0003020522,0.00039440583,0.0018744762,0.00026711787,0.00077963644,0.0003972133,0.00026089192,0.0008744968],"category_scores_gemma":[0.0050340374,0.00017813213,0.0003092398,0.0010812058,0.00040376396,0.00071488216,0.00075392233,0.00022586081,0.00041916754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020620158,0.000059472597,0.83312273,0.00024323862,0.00021030824,0.0002987846,0.0006587692,0.03674432,0.050425787,0.020864028,0.0006173927,0.05654896],"study_design_scores_gemma":[0.000010625373,0.00010611089,0.8344731,0.00004349752,0.00006323441,0.0004945602,0.00019966181,0.12246404,0.022560356,0.014054564,0.0054673515,0.00006298854],"about_ca_topic_score_codex":0.0017496353,"about_ca_topic_score_gemma":0.0014740068,"teacher_disagreement_score":0.0018744762,"about_ca_system_score_codex":0.0004254642,"about_ca_system_score_gemma":0.00033452088,"threshold_uncertainty_score":0.006327331},"labels":[],"label_agreement":null},{"id":"W3103555894","doi":"10.3847/1538-4357/aad80d","title":"The Evolution of Environmental Quenching Timescales to z ∼ 1.6: Evidence for Dynamically Driven Quenching of the Cluster Galaxy Population","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University; University of Toronto; York University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Quenching (fluorescence); Cluster (spacecraft); Star formation; Galaxy cluster; Halo; Population; Accretion (finance); Fluorescence","score_opus":0.007312342035617243,"score_gpt":0.2313699590609625,"score_spread":0.22405761702534527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3103555894","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996178,0.000023698796,0.000076183074,0.000008667977,4.351171e-7,0.0000017398993,0.00008489204,0.000008569052,0.00017791482],"genre_scores_gemma":[0.9998068,0.0000065978866,0.00003650156,0.0000038900102,9.729933e-7,0.0000011831772,0.00010635723,0.0000021811288,0.00003549766],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998708,0.000009061684,0.000004972051,0.00004698283,0.000023339644,0.00004482064],"domain_scores_gemma":[0.9980065,0.0002806395,0.00092294463,0.00014286798,0.0002090811,0.00043793255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041737247,0.00013996655,0.00023596003,0.00082595693,0.0002793816,0.0005137814,0.00036553913,0.0002716157,0.0008922666],"category_scores_gemma":[0.002277671,0.00015481384,0.00021211902,0.00043706602,0.0003614651,0.00029662575,0.00051915017,0.00028970587,0.00014709462],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015168676,0.000023668046,0.9835437,0.000009932461,0.000038408423,0.00004623662,0.00029478336,0.001266317,0.011639571,0.00029520618,0.0001049769,0.0025855193],"study_design_scores_gemma":[0.0000015702362,0.0000135374385,0.9988888,5.818675e-7,0.0000029751025,0.000013910031,0.00001849232,0.00071118976,0.00027100893,0.00003081528,0.0000451217,0.0000020583675],"about_ca_topic_score_codex":0.007964982,"about_ca_topic_score_gemma":0.0067154504,"teacher_disagreement_score":0.007964982,"about_ca_system_score_codex":0.00058411126,"about_ca_system_score_gemma":0.0001419684,"threshold_uncertainty_score":0.015837193},"labels":[],"label_agreement":null},{"id":"W3103650598","doi":"10.3847/1538-4357/abcc69","title":"Discovery of a Low-redshift Damped Lyα System in a Foreground Extended Disk Using a Starburst Galaxy Background Illuminator","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Toronto Rehabilitation Institute","funders":"","keywords":"Redshift; Galaxy; Measure (data warehouse); Offset (computer science); Star formation; Limiting; Quasar","score_opus":0.015731418880256757,"score_gpt":0.25463250062807846,"score_spread":0.2389010817478217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3103650598","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990872,0.000081144986,0.00039583602,0.00001733218,0.0000025048653,0.0000049213,0.00008163943,0.000021863112,0.00030748203],"genre_scores_gemma":[0.9994591,0.0000199481,0.00032111965,0.00001415659,0.0000028998597,0.0000014900658,0.00009544401,0.000002290799,0.000083606006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987435,0.000008989252,0.000008802388,0.00004298351,0.000038399947,0.000026484553],"domain_scores_gemma":[0.99949336,0.00004825721,0.00015816292,0.000047708327,0.00006105853,0.00019158257],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020762875,0.00025714785,0.0002804157,0.00087767735,0.00041011444,0.000689171,0.0003723,0.00033386645,0.00091303774],"category_scores_gemma":[0.00042630598,0.00021038279,0.00015218939,0.00038934246,0.00031543057,0.00019270004,0.0005717136,0.00025415374,0.00029209405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003445179,0.00008255885,0.7481797,0.00004689665,0.000066084816,0.0035959757,0.0003399574,0.00025591045,0.23982143,0.0001827858,0.00018553327,0.0068985536],"study_design_scores_gemma":[0.000019524814,0.00029006464,0.9758221,0.000011070715,0.00004394525,0.005428566,0.000267214,0.001864004,0.014854851,0.00016850016,0.0012171925,0.000012858652],"about_ca_topic_score_codex":0.0012638728,"about_ca_topic_score_gemma":0.0017436036,"teacher_disagreement_score":0.0012638728,"about_ca_system_score_codex":0.0002657046,"about_ca_system_score_gemma":0.00007192958,"threshold_uncertainty_score":0.0030543804},"labels":[],"label_agreement":null},{"id":"W3104010067","doi":"10.3847/1538-4357/abbc04","title":"A 3D Parametric Martian Bow Shock Model with the Effects of Mach Number, Dynamic Pressure, and the Interplanetary Magnetic Field","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"","keywords":"Physics; Bow shock (aerodynamics); Martian; Solar wind; Interplanetary magnetic field; Mach number; Shock (circulatory); Heliosphere; Dynamic pressure; Shock wave; Astrophysics; Geophysics; Mars Exploration Program; Magnetic field; Mechanics; Astronomy","score_opus":0.0027815797122028195,"score_gpt":0.18524824628654257,"score_spread":0.18246666657433974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104010067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97777724,0.00008272132,0.014010118,0.00017348057,0.000022592892,0.000033000808,0.0004357792,0.00014456894,0.007320548],"genre_scores_gemma":[0.9964323,0.000051766543,0.002348618,0.000024199957,0.000007874249,0.000031233318,0.00015847768,0.00001680655,0.00092879724],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999074,0.000024175195,0.0000043671353,0.000017567896,0.000018318733,0.000028123637],"domain_scores_gemma":[0.9997352,0.000098227196,0.000046448207,0.00002507402,0.00004370623,0.000051252908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018186615,0.00051835756,0.0005970621,0.00039286018,0.00048620813,0.0010404002,0.0010976959,0.0010898623,0.0018461234],"category_scores_gemma":[0.0006413067,0.0003564563,0.00075559603,0.00041153686,0.0006128878,0.000613357,0.00082541956,0.00063522207,0.00017190691],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034132805,0.000016674294,0.0010864278,0.0000061388882,0.000011653564,0.0000697036,0.000018164259,0.9971251,0.00054273184,0.00060237525,0.000057375564,0.00042961558],"study_design_scores_gemma":[0.000016945483,0.000018894969,0.000296135,0.0000012614612,0.000004561711,0.0000088334145,0.000012902539,0.99924576,0.000121671685,0.00018054544,0.000088085435,0.0000044158037],"about_ca_topic_score_codex":0.015837742,"about_ca_topic_score_gemma":0.0048060087,"teacher_disagreement_score":0.015837742,"about_ca_system_score_codex":0.0005288036,"about_ca_system_score_gemma":0.00053579354,"threshold_uncertainty_score":0.0314911},"labels":[],"label_agreement":null},{"id":"W3104305329","doi":"10.1086/510997","title":"Anisotropic Galactic Outflows and Enrichment of the Intergalactic Medium. I. Monte Carlo Simulations","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Galaxy; Galaxy formation and evolution; Intergalactic travel; Redshift; Star formation; Structure formation; Context (archaeology); Active galactic nucleus; Universe; Anisotropy; Astronomy","score_opus":0.007219143378722911,"score_gpt":0.22598300271329383,"score_spread":0.21876385933457093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104305329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8006982,0.00063440576,0.17322329,0.0008417521,0.00010469547,0.00019225561,0.0013877525,0.0006343162,0.02228327],"genre_scores_gemma":[0.9647459,0.00029122797,0.030570995,0.00020903752,0.00003122417,0.000158308,0.0005788369,0.0001130314,0.0033015641],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996935,0.000108249216,0.00001455588,0.000051416926,0.000050828276,0.000081393395],"domain_scores_gemma":[0.99890304,0.0004906132,0.00021062662,0.00010816011,0.00016800851,0.00011948007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008125756,0.00054396875,0.0007536562,0.0007838304,0.0007746938,0.001399385,0.0016186206,0.0019692248,0.002451571],"category_scores_gemma":[0.0032993285,0.0005584126,0.0009078809,0.00086722866,0.00083700905,0.0011974867,0.0006981751,0.00090283115,0.00033225756],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023047343,0.000025220388,0.0034288869,0.000009362181,0.000015044824,0.00003526205,0.000022589307,0.98968947,0.00044876055,0.0055146846,0.00012610435,0.0006616164],"study_design_scores_gemma":[0.00001656061,0.0000077063,0.00044107775,0.0000045920674,0.0000051638763,0.000011646544,0.000008747818,0.9973803,0.00018490427,0.0015747605,0.00035869627,0.0000057021316],"about_ca_topic_score_codex":0.026968462,"about_ca_topic_score_gemma":0.012539883,"teacher_disagreement_score":0.026968462,"about_ca_system_score_codex":0.0019010992,"about_ca_system_score_gemma":0.0011426933,"threshold_uncertainty_score":0.05362296},"labels":[],"label_agreement":null},{"id":"W3104342212","doi":"10.1088/0004-637x/723/2/1065","title":"THE BLAST SURVEY OF THE VELA MOLECULAR CLOUD: DYNAMICAL PROPERTIES OF THE DENSE CORES IN VELA-D","year":2010,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Vela; Physics; Astrophysics; Molecular cloud; Galactic plane; Astronomy; Stars; Pulsar","score_opus":0.00902417928870553,"score_gpt":0.21749060290477795,"score_spread":0.20846642361607243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104342212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960097,0.00015359513,0.0001982147,0.0001557215,0.000009501229,0.000009035477,0.0011243139,0.000024161382,0.0023156358],"genre_scores_gemma":[0.99668944,0.00010887489,0.00021314107,0.00006887844,0.000022419808,0.0000077946515,0.0014734939,0.000011825974,0.0014039909],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999923,0.0000072631997,0.0000027020092,0.00001895197,0.00001845907,0.000029531091],"domain_scores_gemma":[0.9997371,0.000027627415,0.00005478994,0.000018077268,0.00004214148,0.00012014348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022326261,0.00016862397,0.00029615665,0.000649186,0.000639468,0.0006221843,0.00024875512,0.00023000245,0.0011438172],"category_scores_gemma":[0.00045024947,0.00018011573,0.00018991994,0.0007182389,0.00020451374,0.00024275744,0.00078523334,0.00038267896,0.0003060052],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033010542,0.00008300674,0.94408023,0.000048205646,0.000103367405,0.0005177717,0.0005964334,0.002865839,0.030575536,0.0007581372,0.0034748092,0.016566593],"study_design_scores_gemma":[0.000012680262,0.000017150898,0.99617094,0.000003898857,0.000011141734,0.00006661951,0.0001259273,0.0014498187,0.0004949748,0.00007124221,0.0015708806,0.000004819554],"about_ca_topic_score_codex":0.02275756,"about_ca_topic_score_gemma":0.032157477,"teacher_disagreement_score":0.02275756,"about_ca_system_score_codex":0.00066378905,"about_ca_system_score_gemma":0.00050228526,"threshold_uncertainty_score":0.045250177},"labels":[],"label_agreement":null},{"id":"W3104441538","doi":"10.3847/1538-4357/abb6f1","title":"Erratum: “A Detailed Observational Analysis of V1324 Sco, the Most Gamma-Ray-luminous Classical Nova to Date” (2018, ApJ, 852, 108)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Nova (rocket); Astrophysics; Astronomy; Aerospace engineering","score_opus":0.030703314760388543,"score_gpt":0.2550518497784846,"score_spread":0.22434853501809607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104441538","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0025964556,0.0017066827,0.0006114545,0.04775399,0.89117223,0.00004402686,0.020417068,0.0009802158,0.03471777],"genre_scores_gemma":[0.02837696,0.006011596,0.0062721204,0.07599073,0.14409894,0.00015860044,0.0592806,0.0042738384,0.67553663],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9985532,0.00009808674,0.00024338457,0.00020901696,0.00075960654,0.00013666693],"domain_scores_gemma":[0.99087673,0.0012910495,0.0007191261,0.00070237566,0.0057065017,0.0007041833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014137379,0.0016060837,0.00087958993,0.0042020963,0.0040104534,0.0031363708,0.0016493788,0.0023229846,0.058549546],"category_scores_gemma":[0.015506844,0.00056344224,0.0007887738,0.0025705306,0.0011020829,0.0021518224,0.0020113518,0.0045039053,0.0441887],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031538628,0.000008397122,0.0002949301,0.00005105812,0.000004523889,0.000112142436,0.000020700196,0.00002169436,0.000088978944,0.00038481434,0.994919,0.0040620975],"study_design_scores_gemma":[0.00002114163,0.000018028739,0.0041419663,0.0002043112,0.000024482868,0.00025001168,0.00013734685,0.000082119055,0.0004129881,0.0008873372,0.99379057,0.000029842355],"about_ca_topic_score_codex":0.032945003,"about_ca_topic_score_gemma":0.049766142,"teacher_disagreement_score":0.058549546,"about_ca_system_score_codex":0.002588857,"about_ca_system_score_gemma":0.0040764534,"threshold_uncertainty_score":0.19586778},"labels":[],"label_agreement":null},{"id":"W3104748327","doi":"10.3847/1538-4357/abd8cd","title":"Revealing Efficient Dust Formation at Low Metallicity in Extragalactic Carbon-rich Wolf-Rayet Binaries","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Metallicity; Binary number; Circumstellar dust; Infrared; Spectroscopy; Star formation; Binary system","score_opus":0.012145891810169982,"score_gpt":0.2349381604710061,"score_spread":0.22279226866083612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3104748327","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99975306,0.0000115553785,0.000026590336,0.0000020010116,2.8272916e-7,9.478088e-7,0.000047744757,0.0000027261551,0.00015509923],"genre_scores_gemma":[0.9996629,0.0000071629834,0.000056100333,0.0000029796438,0.0000010223085,0.0000010274164,0.0001923964,9.948844e-7,0.00007547188],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994254,0.000004529282,0.000004022238,0.000017351653,0.000013304075,0.00001820749],"domain_scores_gemma":[0.9998216,0.000012230451,0.00006247326,0.00001315564,0.000019131086,0.00007144263],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009364976,0.00016740402,0.00017228795,0.0008932125,0.0003191534,0.0003918613,0.0001692698,0.0001583201,0.00087467354],"category_scores_gemma":[0.00017913998,0.000093906856,0.00010537771,0.00037987492,0.0001549116,0.00016472519,0.00038359515,0.000102361526,0.000191785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013869409,0.00003031454,0.95915526,0.000008663355,0.000018675428,0.00019412326,0.000092425515,0.000121388905,0.038208738,0.000038223057,0.000046072626,0.0019475252],"study_design_scores_gemma":[0.0000022081842,0.00002451071,0.99878997,7.099121e-7,0.000003334262,0.00007572378,0.000052451534,0.00016336274,0.0008169404,0.000011751117,0.000058217956,7.7316116e-7],"about_ca_topic_score_codex":0.0016540643,"about_ca_topic_score_gemma":0.0033258372,"teacher_disagreement_score":0.0016540643,"about_ca_system_score_codex":0.00018565275,"about_ca_system_score_gemma":0.00006589248,"threshold_uncertainty_score":0.0032889247},"labels":[],"label_agreement":null},{"id":"W3105335397","doi":"10.3847/1538-4357/ac110b","title":"Igniting Weak Interactions in Neutron Star Postmerger Accretion Disks","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"Syracuse University","keywords":"Neutron star; Parameter space; Kilonova; Accretion (finance); Observable; Ejecta; Neutrino; Nucleosynthesis; Black hole (networking)","score_opus":0.019836388415278454,"score_gpt":0.26818948659308356,"score_spread":0.2483530981778051,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3105335397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974923,0.00004555016,0.00066548487,0.000048829712,0.000005089065,0.000005339768,0.00003663152,0.000028558792,0.0016720819],"genre_scores_gemma":[0.99950635,0.00002374076,0.0002066698,0.0000124931175,0.000002739228,0.000004552708,0.000030722178,0.00000889491,0.00020381952],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999031,0.000020138341,0.0000043254604,0.000011320614,0.00001885011,0.00004230005],"domain_scores_gemma":[0.99945456,0.00024902492,0.0001101148,0.000029146811,0.000036926598,0.00012025257],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028484256,0.00043493864,0.00047965668,0.0004183787,0.0007417246,0.0011846167,0.00080908067,0.0007480828,0.0012187951],"category_scores_gemma":[0.0014206262,0.00035387857,0.0005310326,0.00022570431,0.00086988154,0.00045992236,0.00073514465,0.00052419875,0.00013793135],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003666252,0.00018304557,0.024968488,0.000055691853,0.00009306381,0.00090960896,0.00020800396,0.9498166,0.01757426,0.004131876,0.00022963746,0.0014631454],"study_design_scores_gemma":[0.00014984256,0.00021020538,0.009696274,0.000010897229,0.000036054138,0.00011720967,0.00015706645,0.9834567,0.0042984197,0.0014718599,0.000372752,0.000022779497],"about_ca_topic_score_codex":0.0074783186,"about_ca_topic_score_gemma":0.003032991,"teacher_disagreement_score":0.0074783186,"about_ca_system_score_codex":0.001141041,"about_ca_system_score_gemma":0.00041810816,"threshold_uncertainty_score":0.014869571},"labels":[],"label_agreement":null},{"id":"W3105731827","doi":"10.1088/0004-637x/771/1/13","title":"A SEARCH FOR RAPIDLY ACCRETING WHITE DWARFS IN THE SMALL MAGELLANIC CLOUD","year":2013,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"White dwarf; Physics; Astrophysics; Supernova; Stars; Astronomy; Photosphere; Nebula; Small Magellanic Cloud; Light curve; Spectral line","score_opus":0.018523674191648416,"score_gpt":0.24324183474741384,"score_spread":0.22471816055576543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3105731827","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998389,0.0002535995,0.00030814132,0.000088637105,0.0000048063994,0.000010751844,0.00012442746,0.000019405254,0.0008012439],"genre_scores_gemma":[0.9979976,0.00015977837,0.00083088566,0.000063977415,0.000018058176,0.0000033180268,0.0004375934,0.0000030155195,0.00048576738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989736,0.0000070503443,0.0000055592845,0.000031654334,0.000030351288,0.000027878988],"domain_scores_gemma":[0.9994772,0.000057319485,0.0001307725,0.000036504003,0.000035125053,0.00026301717],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000219793,0.00020682496,0.00027140524,0.0011308603,0.0006662939,0.00065338204,0.00036498057,0.0004150522,0.0014668565],"category_scores_gemma":[0.00043458102,0.00012660708,0.00017797205,0.000978833,0.00024131077,0.0004112668,0.00041538544,0.00017817902,0.00040300295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010640835,0.00009002348,0.94536835,0.00006338107,0.000038534174,0.0009396125,0.00029093603,0.000101910504,0.030538578,0.0005025006,0.00049341784,0.021466352],"study_design_scores_gemma":[0.000008591863,0.00015670317,0.9928558,0.000014071939,0.000023742698,0.0014457066,0.00046769984,0.00047309112,0.0021538273,0.0002858095,0.0021082684,0.000006578487],"about_ca_topic_score_codex":0.0023587605,"about_ca_topic_score_gemma":0.0048853196,"teacher_disagreement_score":0.0023587605,"about_ca_system_score_codex":0.00017854723,"about_ca_system_score_gemma":0.00032521438,"threshold_uncertainty_score":0.004907191},"labels":[],"label_agreement":null},{"id":"W3106255192","doi":"10.3847/1538-4357/aab359","title":"A Serendipitous MWA Search for Narrowband Signals from ‘Oumuamua","year":2018,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Space Science and Extraterrestrial Life","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Search for extraterrestrial intelligence; Spacecraft; Narrowband; Physics; Broadband; Remote sensing; Astronomy; Aerospace engineering; Engineering; Optics; Geography","score_opus":0.028432466959532235,"score_gpt":0.29687060738245524,"score_spread":0.268438140422923,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3106255192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976954,0.0000810883,0.0005232761,0.000058623067,0.000008115053,0.0000025491108,0.00012686395,0.000024991905,0.0014792276],"genre_scores_gemma":[0.99809355,0.000028106748,0.001001769,0.000046888137,0.000015395837,0.000005005199,0.00035684515,0.0000056226795,0.0004467783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998789,0.000015937283,0.000004751611,0.000034079654,0.000036223082,0.000030099061],"domain_scores_gemma":[0.99946016,0.00014349395,0.00013420093,0.00006769512,0.00009262448,0.000101960024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020539627,0.00012259893,0.0001855043,0.0010536164,0.0005945428,0.00034149294,0.00027524447,0.0003027964,0.0012495492],"category_scores_gemma":[0.0005774818,0.00010833286,0.00013077554,0.00063523906,0.00026266548,0.00021542441,0.00047890766,0.00030847715,0.00019105912],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051477016,0.000112849986,0.8350882,0.000070375674,0.00015110275,0.0012211773,0.0018409557,0.00041007056,0.11482142,0.00039996378,0.0019285536,0.04344048],"study_design_scores_gemma":[0.000010174384,0.000106843516,0.98781514,0.0000106159705,0.000039567596,0.00047322735,0.0006152417,0.0006083085,0.006638141,0.00011916618,0.003552651,0.000010939073],"about_ca_topic_score_codex":0.003334144,"about_ca_topic_score_gemma":0.008600374,"teacher_disagreement_score":0.003334144,"about_ca_system_score_codex":0.000194828,"about_ca_system_score_gemma":0.00013289333,"threshold_uncertainty_score":0.006629467},"labels":[],"label_agreement":null},{"id":"W3106411158","doi":"10.3847/1538-4357/ac0891","title":"Rapid Variability of Sgr A* across the Electromagnetic Spectrum","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Sagittarius A*; Accretion (finance); Synchrotron radiation; Galactic Center; Computational physics; Galaxy; Optics","score_opus":0.009571795922356744,"score_gpt":0.2341638847432534,"score_spread":0.22459208882089665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3106411158","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986688,0.00003036831,0.0002878568,0.000016698468,0.0000028692134,0.0000017238585,0.0004006595,0.000035128287,0.0005559894],"genre_scores_gemma":[0.99914455,0.000008756267,0.00011989972,0.0000067748742,0.0000030246797,0.0000013663836,0.0006194169,0.0000046822142,0.00009155566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999902,0.000018831115,0.000006874214,0.00003943787,0.000018363256,0.000014430458],"domain_scores_gemma":[0.9996674,0.000058454665,0.00010132322,0.00004230331,0.000060948318,0.000069661546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023755622,0.00015430908,0.00012462746,0.000633177,0.0001579823,0.00042050987,0.00013572576,0.00016525017,0.0006024885],"category_scores_gemma":[0.00046191903,0.000091585214,0.00022049341,0.00039516643,0.00012915075,0.00017901039,0.0003041748,0.00015683303,0.0003020286],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013555678,0.000047056048,0.94631463,0.000016033133,0.000121505356,0.0001438714,0.00013549371,0.0015233756,0.042171463,0.00031318192,0.000623274,0.008454493],"study_design_scores_gemma":[0.0000020665975,0.00002003981,0.99769884,8.772567e-7,0.000004883332,0.000045894463,0.000024811294,0.0013194161,0.00049536466,0.000051439325,0.00033384844,0.0000025700976],"about_ca_topic_score_codex":0.0022129505,"about_ca_topic_score_gemma":0.0017035974,"teacher_disagreement_score":0.0022129505,"about_ca_system_score_codex":0.00013609757,"about_ca_system_score_gemma":0.000055999564,"threshold_uncertainty_score":0.004400134},"labels":[],"label_agreement":null},{"id":"W3107335719","doi":"10.3847/1538-4357/abcda4","title":"Ancient Very Metal-poor Stars Associated with the Galactic Disk in the H3 Survey","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Stars; Galaxy; Population; Accretion (finance); Thick disk; Angular momentum; Star formation","score_opus":0.020835802990578016,"score_gpt":0.26714297587768515,"score_spread":0.24630717288710713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3107335719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990637,0.000057472258,0.000057372756,0.000010905793,7.656791e-7,0.000001553079,0.0005325389,0.000005077743,0.00027072802],"genre_scores_gemma":[0.9991474,0.00003973969,0.00007693307,0.0000103134,0.0000018661702,0.0000016092058,0.0006358678,0.0000027500153,0.00008338353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998524,0.000019204137,0.00001169728,0.00004601204,0.000031840438,0.0000388835],"domain_scores_gemma":[0.9993266,0.000055476794,0.00029120478,0.00007817471,0.00009683845,0.00015172872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021461662,0.00014393916,0.00019842888,0.0007986512,0.00028376753,0.0004465279,0.00020578146,0.00018485998,0.00067268644],"category_scores_gemma":[0.0004830797,0.00009665439,0.00016087467,0.00090677006,0.00023038675,0.00025766398,0.00047150216,0.00016113106,0.0002717719],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029792262,0.00000438981,0.9970271,0.000004219099,0.000012271192,0.000024679888,0.00006795425,0.000023641524,0.0015530604,0.000014884238,0.00006150946,0.0011764306],"study_design_scores_gemma":[6.6034255e-7,0.0000058550245,0.9995022,0.0000011292493,0.0000033998801,0.000053079806,0.00006885159,0.000039553262,0.0001680442,0.000006937693,0.00014981467,5.813581e-7],"about_ca_topic_score_codex":0.011969097,"about_ca_topic_score_gemma":0.018118065,"teacher_disagreement_score":0.011969097,"about_ca_system_score_codex":0.0002718297,"about_ca_system_score_gemma":0.00015735583,"threshold_uncertainty_score":0.023798823},"labels":[],"label_agreement":null},{"id":"W3108405318","doi":"10.3847/1538-4357/abccd9","title":"The Radio Luminosity-risetime Function of Core-collapse Supernovae","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Supernova; Luminosity; Flux (metallurgy); Type (biology); Standard deviation; Spectral line; Luminosity function; Erg","score_opus":0.011838161557605354,"score_gpt":0.22296947527097222,"score_spread":0.21113131371336685,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3108405318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955456,0.00020410596,0.002137859,0.000013362618,0.0000024418896,0.0000067012734,0.0008395907,0.00011358345,0.0011366964],"genre_scores_gemma":[0.9971476,0.00005818079,0.0005794772,0.0000073265596,0.000005968574,0.000006047644,0.0018348965,0.000021606202,0.00033884408],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997899,0.000042756823,0.000016171898,0.000053423097,0.000055936227,0.000041883995],"domain_scores_gemma":[0.99694234,0.0011998927,0.0009533319,0.00030588903,0.0003612247,0.00023732727],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011708044,0.00039711752,0.00023644062,0.0023069135,0.00013732006,0.0006784222,0.00030070235,0.00024975944,0.0013279319],"category_scores_gemma":[0.0035687976,0.00024562835,0.00048765974,0.0007118738,0.00020754244,0.00043799632,0.00036023857,0.00027172785,0.00064311596],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018993876,0.000058005444,0.9593884,0.000047175276,0.0001485649,0.00011047651,0.00012283675,0.00869072,0.01868556,0.0005065751,0.000303961,0.011747773],"study_design_scores_gemma":[0.0000032261332,0.00004587418,0.9893142,0.0000040187456,0.000013668146,0.00012726735,0.000018495151,0.009062781,0.0009527505,0.00013170471,0.00031862006,0.0000072895873],"about_ca_topic_score_codex":0.0019248722,"about_ca_topic_score_gemma":0.0015487942,"teacher_disagreement_score":0.0023069135,"about_ca_system_score_codex":0.0003257422,"about_ca_system_score_gemma":0.00009740644,"threshold_uncertainty_score":0},"labels":[],"label_agreement":null},{"id":"W3108480225","doi":"10.3847/1538-4357/abe7e6","title":"A Search for Time-dependent Astrophysical Neutrino Emission with IceCube Data from 2012 to 2017","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Physics; Neutrino; Neutrino astronomy; Astrophysics; Astronomy; Neutrino detector; Nuclear physics; Neutrino oscillation","score_opus":0.025307454110713497,"score_gpt":0.27463549879282934,"score_spread":0.24932804468211583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3108480225","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9762418,0.00024627234,0.00063306233,0.00009069933,0.000017567263,0.00002587355,0.020389376,0.00005003436,0.0023051468],"genre_scores_gemma":[0.9295006,0.00025715778,0.0015655954,0.00003485447,0.000042369753,0.000056045006,0.06769298,0.000043305496,0.0008071486],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962807,0.00006684044,0.00001929193,0.00013005505,0.00007305166,0.00008263632],"domain_scores_gemma":[0.9991762,0.00022654867,0.00026562743,0.00009817265,0.00012780534,0.00010562061],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072218024,0.00024442197,0.00036544175,0.0017865773,0.00024735785,0.00074802694,0.0002739496,0.00027412464,0.0013664431],"category_scores_gemma":[0.0011559261,0.000104668376,0.00046891993,0.0019537255,0.00024079435,0.00026891424,0.00056277885,0.00024287342,0.00035097805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001332201,0.00018200789,0.94825864,0.00021380381,0.00061940216,0.0007361415,0.00037950889,0.007409888,0.013104938,0.0011859852,0.0078012366,0.018776326],"study_design_scores_gemma":[0.000036143334,0.000092638445,0.98119694,0.000042117314,0.00011841216,0.00027492322,0.00030129057,0.0055236975,0.003369845,0.0002190385,0.008806135,0.000018771885],"about_ca_topic_score_codex":0.011796795,"about_ca_topic_score_gemma":0.014921368,"teacher_disagreement_score":0.011796795,"about_ca_system_score_codex":0.00043920233,"about_ca_system_score_gemma":0.000581559,"threshold_uncertainty_score":0.023456275},"labels":[],"label_agreement":null},{"id":"W3108529847","doi":"10.3847/1538-4357/abceb6","title":"Resolving the Dust-to-Metals Ratio and CO-to-H<sub>2</sub> Conversion Factor in the Nearby Universe","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"European Research Council; Deutsche Forschungsgemeinschaft; National Science Foundation","keywords":"Metallicity; Astrophysics; Physics; Galaxy; Interstellar medium; Emissivity; Black-body radiation; Line (geometry); Cosmic dust; Density ratio; Optics; Geometry; Radiation","score_opus":0.012622369040956637,"score_gpt":0.2374031238368393,"score_spread":0.22478075479588266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3108529847","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991918,0.000036391055,0.00047546948,0.000007984576,4.913034e-7,0.0000016966876,0.00005051791,0.000025840636,0.00020977027],"genre_scores_gemma":[0.999522,0.000008864325,0.00035955734,0.000002931438,0.0000010623418,7.3356927e-7,0.00007268217,0.000002370433,0.00002979319],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987423,0.000017931814,0.000005077793,0.000050564322,0.000026291882,0.000025790017],"domain_scores_gemma":[0.9995834,0.00012217076,0.00010357232,0.00006959964,0.000044157194,0.00007707182],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003618473,0.00036057545,0.00021064872,0.00074760785,0.0002180532,0.00057270844,0.00034247982,0.0003032829,0.0005858587],"category_scores_gemma":[0.0008781441,0.0002372122,0.00027098277,0.00043581,0.00018984788,0.00023497759,0.00032491688,0.00018161454,0.0001613609],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003126849,0.000062826715,0.9035753,0.000029004259,0.00016642635,0.00023354402,0.00012184352,0.01202938,0.0758184,0.00029381784,0.00015523298,0.0072014704],"study_design_scores_gemma":[0.000018697627,0.00008151544,0.95824534,0.0000036269341,0.000055769564,0.000097536,0.00010879724,0.029196022,0.01169748,0.00018813166,0.00029468889,0.000012461603],"about_ca_topic_score_codex":0.006466126,"about_ca_topic_score_gemma":0.0069551715,"teacher_disagreement_score":0.006466126,"about_ca_system_score_codex":0.00041280617,"about_ca_system_score_gemma":0.000115456685,"threshold_uncertainty_score":0.01285696},"labels":[],"label_agreement":null},{"id":"W3109050538","doi":"10.3847/1538-4357/abc47b","title":"Faint Quasars Live in the Same Number Density Environments as Lyman Break Galaxies at z ∼ 4","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; Science Mission Directorate; Japan Society for the Promotion of Science; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Eötvös Loránd Tudományegyetem; Academia Sinica; Space Telescope Science Institute; Queen's University; Ministry of Education, Culture, Sports, Science and Technology; Los Alamos National Laboratory; Princeton University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Smithsonian Institution; Japan Science and Technology Agency; Cabinet Office, Government of Japan; Durham University; National Science Foundation","keywords":"Quasar; Galaxy; Sky; OVV quasar; Number density; Galaxy formation and evolution","score_opus":0.009026293420656684,"score_gpt":0.21037870008458123,"score_spread":0.20135240666392454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3109050538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992545,0.000056667704,0.00011513286,0.000016382626,0.0000014159327,0.000001609785,0.00006945251,0.0000057565057,0.0004789731],"genre_scores_gemma":[0.99975246,0.000020870304,0.000033641856,0.000007693778,0.0000029644175,6.934465e-7,0.00008519678,8.773889e-7,0.00009556895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998252,0.00001678634,0.0000086407945,0.00004941767,0.000031308304,0.00006877525],"domain_scores_gemma":[0.9989121,0.000104078834,0.0005929772,0.00007297073,0.00007954122,0.00023831244],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022541569,0.00012998644,0.00020131278,0.0010182875,0.00042687776,0.00090450875,0.00025027193,0.00015668148,0.0030159946],"category_scores_gemma":[0.0008214153,0.00012736727,0.00014369068,0.00045032823,0.0005846803,0.0005455964,0.00052211306,0.00022174555,0.00028921023],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004586478,0.0000085093,0.994351,0.0000035272603,0.000026509586,0.000042583273,0.00010933709,0.0000620364,0.0035222168,0.00018876033,0.000063283675,0.0015763509],"study_design_scores_gemma":[0.0000014495928,0.000013824971,0.99937785,0.0000011003569,0.0000061211767,0.00005850939,0.00016689487,0.000062746156,0.00014589976,0.00005847118,0.0001058947,0.0000012114735],"about_ca_topic_score_codex":0.0058773314,"about_ca_topic_score_gemma":0.008620905,"teacher_disagreement_score":0.0058773314,"about_ca_system_score_codex":0.00024315425,"about_ca_system_score_gemma":0.00012854394,"threshold_uncertainty_score":0.0116862655},"labels":[],"label_agreement":null},{"id":"W3109088998","doi":"10.3847/1538-4357/abe40e","title":"One Channel to Rule Them All? Constraining the Origins of Binary Black Holes Using Multiple Formation Pathways","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":305,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Fonds Wetenschappelijk Onderzoek; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; European Commission; Space Telescope Science Institute; Canadian Institute for Advanced Research; University of Chicago; Northwestern University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Binary number; Channel (broadcasting); Population; Spins; Binary black hole; Range (aeronautics)","score_opus":0.06850638519785722,"score_gpt":0.3208075316054887,"score_spread":0.25230114640763146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3109088998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9657984,0.00042544957,0.030103575,0.0003443134,0.000021953078,0.000013617437,0.0003664542,0.00015208228,0.0027740533],"genre_scores_gemma":[0.9969311,0.00007450407,0.0027099806,0.000024616633,0.000009706339,0.0000028830345,0.00013170687,0.000025270336,0.00009023663],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995921,0.00013500405,0.000021620413,0.000115481926,0.00006589808,0.00006990412],"domain_scores_gemma":[0.9952485,0.0027968185,0.0008291581,0.0005310307,0.00023406689,0.00036042943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025617785,0.00043026273,0.0004942884,0.001372108,0.00053092535,0.0029907352,0.0006686007,0.0005132875,0.0025122424],"category_scores_gemma":[0.012100989,0.0002620149,0.0005758376,0.00069477316,0.0007108397,0.0022267776,0.0013251909,0.00039198535,0.00028965835],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002677686,0.00006743053,0.80750513,0.00012349,0.00025563943,0.00024158994,0.00022695902,0.09580877,0.0039810482,0.053540114,0.0015620674,0.036419984],"study_design_scores_gemma":[0.000053766034,0.000074743904,0.17036948,0.00014173746,0.00026029514,0.00033167837,0.0005686534,0.7263163,0.005978062,0.09123725,0.004599392,0.00006865103],"about_ca_topic_score_codex":0.002478439,"about_ca_topic_score_gemma":0.0023578776,"teacher_disagreement_score":0.0029907352,"about_ca_system_score_codex":0.00040783876,"about_ca_system_score_gemma":0.0004631909,"threshold_uncertainty_score":0.013548136},"labels":[],"label_agreement":null},{"id":"W3110874471","doi":"10.3847/1538-4357/abc332","title":"Searching for Nuclear Obscuration in the Infrared Spectra of Nearby FR I Radio Galaxies","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Torus; Active galactic nucleus; Galaxy; Infrared; Photometry (optics); Radio galaxy; Spectral line; Luminous infrared galaxy; Quasar","score_opus":0.013540344331294347,"score_gpt":0.22316497978996044,"score_spread":0.2096246354586661,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3110874471","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99908483,0.000014149818,0.0007062879,0.000005914841,2.5775182e-7,0.0000017911515,0.00003451052,0.000011294363,0.00014104771],"genre_scores_gemma":[0.99960977,0.000007323192,0.0002999474,0.000001839998,7.982657e-7,8.7724356e-7,0.000057407073,0.0000014527888,0.000020652795],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998301,0.000042466112,0.000010144438,0.00005330128,0.000035468132,0.000028456749],"domain_scores_gemma":[0.9981857,0.0007988291,0.00062328554,0.00013672495,0.000100830424,0.00015471099],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006515877,0.00018584562,0.00018587681,0.0008745493,0.00021836383,0.00046788028,0.00037669318,0.00024316701,0.0008149857],"category_scores_gemma":[0.002386142,0.00018884336,0.00033031014,0.00037180804,0.00040227003,0.00034479584,0.00023358419,0.0001786431,0.00013559122],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005851041,0.000021087242,0.9846144,0.0000055450005,0.000034135395,0.00006606568,0.00010964112,0.007909511,0.004706295,0.00017445572,0.000027200058,0.0022732362],"study_design_scores_gemma":[0.0000056352264,0.000102749575,0.9488476,0.000004750222,0.000024828669,0.00015753604,0.00014234151,0.048900135,0.0014430144,0.00026283704,0.00009924243,0.000009381002],"about_ca_topic_score_codex":0.007673525,"about_ca_topic_score_gemma":0.007886815,"teacher_disagreement_score":0.007673525,"about_ca_system_score_codex":0.00037819994,"about_ca_system_score_gemma":0.00010802546,"threshold_uncertainty_score":0.015257716},"labels":[],"label_agreement":null},{"id":"W3111196359","doi":"10.3847/1538-4357/abf24a","title":"The Cepheid Distance to the Narrow-line Seyfert 1 Galaxy NGC 4051","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"California Institute of Technology; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Cepheid variable; Physics; Galaxy; Astrophysics; Astronomy; Hubble sequence; Line (geometry); Cosmic distance ladder; Luminous infrared galaxy; Stars","score_opus":0.010087468097200274,"score_gpt":0.22927572195175408,"score_spread":0.21918825385455382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111196359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99732095,0.00013328531,0.00015976555,0.000035713096,0.000003165669,0.0000012267288,0.00024825713,0.0000047638173,0.00209278],"genre_scores_gemma":[0.99906045,0.00008117129,0.00013214284,0.0000068039894,0.0000036703439,0.0000014929328,0.00032525108,0.0000013960407,0.00038751593],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992096,0.000008134606,0.0000039499273,0.000025041183,0.000022711929,0.000019096657],"domain_scores_gemma":[0.9995735,0.000083675164,0.00014973195,0.00003816488,0.00006460702,0.00009028016],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020609816,0.00014625909,0.00012660211,0.0011120702,0.0005402245,0.0004826942,0.00023309718,0.0001635896,0.0024441495],"category_scores_gemma":[0.00078785216,0.000064823915,0.00008287722,0.00047664603,0.0002834374,0.00026556154,0.00041640777,0.00018981604,0.0004481178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059910806,0.000014292736,0.9783815,0.00003281326,0.000027833756,0.00017232315,0.0003971206,0.0012590594,0.0041319635,0.0020601002,0.0005621482,0.012900774],"study_design_scores_gemma":[0.0000020834034,0.000009847042,0.99766904,0.000007722415,0.0000058912474,0.00008326514,0.00012836873,0.00042722662,0.00037476397,0.00026671976,0.0010223974,0.000002616749],"about_ca_topic_score_codex":0.011450673,"about_ca_topic_score_gemma":0.0154057145,"teacher_disagreement_score":0.011450673,"about_ca_system_score_codex":0.0005439213,"about_ca_system_score_gemma":0.00016780019,"threshold_uncertainty_score":0.02276808},"labels":[],"label_agreement":null},{"id":"W3111196955","doi":"10.3847/1538-4357/abd2c3","title":"Swift Multiwavelength Follow-up of LVC S200224ca and the Implications for Binary Black Hole Mergers","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council; Ministero degli Affari Esteri e della Cooperazione Internazionale; Türkiye Bilimsel ve Teknolojik Araştırma Kurumu; Nuclear Safety and Security Commission; Ministero dell’Istruzione, dell’Università e della Ricerca; Villum Fonden; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Swift; Binary number; Binary black hole; Astronomy; Gravitational wave","score_opus":0.017576931215536,"score_gpt":0.2517560754638695,"score_spread":0.23417914424833353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111196955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997361,0.00013134388,0.00007874025,0.00022333421,0.000008662134,0.000005033048,0.00030729547,0.000010743406,0.0018737693],"genre_scores_gemma":[0.99920386,0.000024372985,0.00006205096,0.0000664839,0.000012854566,0.0000022634545,0.00034950618,0.0000042907745,0.00027432505],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985707,0.000016196122,0.000008520622,0.000037111495,0.00003239142,0.000048768507],"domain_scores_gemma":[0.9991523,0.00012096407,0.0003586307,0.000061116676,0.00011689986,0.00019013738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037271783,0.00016560902,0.00024229658,0.0008957769,0.00068780297,0.0010317247,0.00033750836,0.00047796435,0.0012638128],"category_scores_gemma":[0.0011262418,0.0001023379,0.00022281348,0.0005987552,0.00028016503,0.00034597743,0.00075316906,0.00044854128,0.000192766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017984134,0.000056962486,0.9868046,0.000012353167,0.000025764288,0.00094541116,0.0002530562,0.00033552194,0.004555845,0.00031872973,0.0008412912,0.0056705633],"study_design_scores_gemma":[0.00000429412,0.000029886374,0.9977245,0.0000071754525,0.000008140249,0.00020847793,0.00019355745,0.0005453069,0.0004081177,0.00015239151,0.0007130883,0.0000051673533],"about_ca_topic_score_codex":0.013804814,"about_ca_topic_score_gemma":0.024679674,"teacher_disagreement_score":0.013804814,"about_ca_system_score_codex":0.00064007536,"about_ca_system_score_gemma":0.00021633542,"threshold_uncertainty_score":0.027448952},"labels":[],"label_agreement":null},{"id":"W3111238147","doi":"10.3847/1538-4357/abfe62","title":"Probing Cosmic Reionization and Molecular Gas Growth with TIME","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Reionization; Galaxy; COSMIC cancer database; Intensity mapping; Star formation; Redshift; Luminosity function; Galaxy formation and evolution; Luminosity","score_opus":0.003259284678024917,"score_gpt":0.17504049216308012,"score_spread":0.1717812074850552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111238147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97322494,0.00025648074,0.022528386,0.00022813676,0.000008057923,0.000010751027,0.0007477745,0.00015520083,0.002840294],"genre_scores_gemma":[0.99682695,0.000070222995,0.0025519894,0.000016777649,0.0000048235556,0.0000044847598,0.00023901276,0.000014183304,0.00027153804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989736,0.000026420908,0.0000030705414,0.00004064904,0.00001654823,0.000015936377],"domain_scores_gemma":[0.99894637,0.00039153334,0.00037021283,0.00012885378,0.00008265664,0.000080337806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061218924,0.00031963998,0.00016707329,0.0005114363,0.00015884539,0.0006437427,0.0004402009,0.0004173898,0.0009834465],"category_scores_gemma":[0.0026823923,0.00017499794,0.00021473021,0.00066681317,0.00033641854,0.001199522,0.00053251727,0.00023491778,0.00012723579],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014944126,0.00007586377,0.7580672,0.000054652108,0.00011217585,0.00014402428,0.00016460533,0.17452775,0.016778514,0.020952443,0.0005999175,0.028373474],"study_design_scores_gemma":[0.000012183347,0.00006117931,0.4606963,0.00002057763,0.00004578615,0.00009732517,0.0000853426,0.5164812,0.008163008,0.011288492,0.0030146802,0.000033966633],"about_ca_topic_score_codex":0.0061148647,"about_ca_topic_score_gemma":0.005399277,"teacher_disagreement_score":0.0061148647,"about_ca_system_score_codex":0.00080754317,"about_ca_system_score_gemma":0.0002193977,"threshold_uncertainty_score":0.012158573},"labels":[],"label_agreement":null},{"id":"W3111252994","doi":"10.3847/1538-4357/ac83a8","title":"Galaxy Alignments with Surrounding Structure in the Sloan Digital Sky Survey","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Center for Cosmology and Astroparticle Physics, Ohio State University; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Sky; Galaxy; Luminosity; Sigma; Luminous infrared galaxy; Galaxy group; Astronomy","score_opus":0.00872649259609374,"score_gpt":0.2095715857141023,"score_spread":0.20084509311800858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111252994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99754035,0.00007387908,0.00009822742,0.000016311193,0.0000017048762,0.000002010401,0.0010971173,0.000013213488,0.0011573412],"genre_scores_gemma":[0.99749064,0.00003191621,0.00011470942,0.0000067001524,0.0000027802296,0.0000022912682,0.002162511,0.0000063973557,0.00018200236],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959475,0.00008558796,0.000028867664,0.00009298516,0.00011989245,0.000078021825],"domain_scores_gemma":[0.9974577,0.00025709183,0.0013403549,0.00025068497,0.00031433915,0.00037988456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041119452,0.00015307704,0.00020159052,0.0016526199,0.00032798148,0.0008967996,0.00014147515,0.00012545481,0.001374989],"category_scores_gemma":[0.0023183369,0.00011417692,0.00018911003,0.0030117892,0.0003678958,0.0003243678,0.00088204595,0.00018321698,0.00039646085],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003593574,0.000006303133,0.99738735,0.000007146692,0.00003567874,0.000015899086,0.0000849573,0.00029313663,0.0004984777,0.000072530944,0.00028878803,0.0012736596],"study_design_scores_gemma":[6.2477113e-7,0.0000028731413,0.99948955,0.0000011077485,0.0000029039609,0.000006123496,0.00004458596,0.00015300624,0.000033404835,0.000012169168,0.0002527441,9.041266e-7],"about_ca_topic_score_codex":0.027231222,"about_ca_topic_score_gemma":0.043409824,"teacher_disagreement_score":0.027231222,"about_ca_system_score_codex":0.00056869216,"about_ca_system_score_gemma":0.00027743517,"threshold_uncertainty_score":0.054145455},"labels":[],"label_agreement":null},{"id":"W3111272849","doi":"10.3847/1538-4357/ac7467","title":"Using LSST Microlensing to Constrain Dark Compact Objects in Spherical and Disk Configurations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Gravitational microlensing; Physics; Dark matter; Astrophysics; Sky; Galaxy; Black hole (networking); Astronomy; Computer science","score_opus":0.014015942910282164,"score_gpt":0.24081267023412345,"score_spread":0.2267967273238413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111272849","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98270583,0.00041420117,0.0101311095,0.00009096719,0.000008272493,0.000010816129,0.0013841286,0.0002888944,0.0049656904],"genre_scores_gemma":[0.99710983,0.000046112236,0.0018552091,0.000017113705,0.000008568502,0.000002134963,0.0008181513,0.000014111547,0.00012871159],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99973875,0.00003923693,0.000010856236,0.000075873606,0.00007289842,0.0000623516],"domain_scores_gemma":[0.9985795,0.00036933963,0.0003339892,0.00018357403,0.00021068654,0.0003228157],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000724535,0.00039017995,0.00023348177,0.0024412794,0.00032795584,0.0016326949,0.00037336058,0.00029476313,0.0014063823],"category_scores_gemma":[0.0022000712,0.0002736562,0.00042311387,0.0009401701,0.0002828875,0.0006966,0.00129859,0.0002836772,0.00040045052],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017767576,0.000031195334,0.9277794,0.000052636384,0.00022376854,0.00022990386,0.00018581127,0.03036781,0.013363283,0.0023227374,0.00079406635,0.024471747],"study_design_scores_gemma":[0.000017514687,0.000049381368,0.7899766,0.000036441867,0.00007368153,0.00023723567,0.00029860332,0.19690028,0.006944673,0.0028475206,0.0025767891,0.000041303065],"about_ca_topic_score_codex":0.012548595,"about_ca_topic_score_gemma":0.014776152,"teacher_disagreement_score":0.012548595,"about_ca_system_score_codex":0.0005741234,"about_ca_system_score_gemma":0.00020260506,"threshold_uncertainty_score":0.0249511},"labels":[],"label_agreement":null},{"id":"W3111289162","doi":"10.3847/1538-4357/abceb5","title":"The Evolution of Magellanic-like Galaxy Pairs and the Production of Magellanic Stream Analogs in Simulations with Tides, Ram Pressure, and Stellar Feedback","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Galaxy; Ram pressure; Dwarf galaxy; Star formation; Metallicity; Tidal force; Stars","score_opus":0.006416085501258052,"score_gpt":0.22866685028571287,"score_spread":0.22225076478445482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111289162","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99570763,0.000043243534,0.0006276244,0.00017483576,0.000022725586,0.000022572855,0.00029785416,0.00007750644,0.0030260773],"genre_scores_gemma":[0.99787307,0.000036557227,0.0009668031,0.00006766101,0.00000901169,0.00003862027,0.00037776792,0.000032439224,0.0005981285],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998204,0.00005433316,0.000008815741,0.000026223335,0.000027852317,0.00006237584],"domain_scores_gemma":[0.99813604,0.00096691033,0.0001656067,0.00010973653,0.00018944289,0.00043218624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006141081,0.0005436943,0.00078127376,0.0006580421,0.0010587646,0.0011299455,0.001381343,0.0014463156,0.0026094376],"category_scores_gemma":[0.0032945166,0.0005315234,0.0008553764,0.0005977582,0.0011945701,0.0007339218,0.0008922283,0.0013155807,0.0002120713],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002903247,0.00034041333,0.025100207,0.000033064596,0.00012895299,0.00025561755,0.00013428785,0.9678022,0.0016154926,0.0023022592,0.0007875149,0.0012097682],"study_design_scores_gemma":[0.00013203899,0.00011596903,0.0047220658,0.000008021736,0.000027372804,0.000021413687,0.00011825993,0.9935928,0.0004133089,0.0005358627,0.0002980066,0.000014837398],"about_ca_topic_score_codex":0.034279175,"about_ca_topic_score_gemma":0.023437755,"teacher_disagreement_score":0.034279175,"about_ca_system_score_codex":0.0016293569,"about_ca_system_score_gemma":0.0011943153,"threshold_uncertainty_score":0.06815928},"labels":[],"label_agreement":null},{"id":"W3111326950","doi":"10.3847/1538-4357/abd3a8","title":"Constraining the Quasar Radio-loud Fraction at z ∼ 6 with Deep Radio Observations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Jansky; Redshift; Population; Fraction (chemistry); OVV quasar; Flux (metallurgy)","score_opus":0.014826407111144387,"score_gpt":0.2141744101412671,"score_spread":0.1993480030301227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111326950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922776,0.00031330553,0.0035071794,0.00006982116,0.0000115005405,0.000011546433,0.0014503641,0.00008262168,0.0022760108],"genre_scores_gemma":[0.99467814,0.00013384497,0.0024130014,0.000046770045,0.00003145534,0.000007014774,0.0020016173,0.000019350355,0.000668755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998323,0.000017269313,0.000008103147,0.000050029306,0.00003223755,0.00006007308],"domain_scores_gemma":[0.9987446,0.00019951517,0.00041244362,0.00013275121,0.00011065187,0.00040011771],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005750763,0.0004833282,0.00028323804,0.0016077315,0.00025586173,0.000844405,0.00032923368,0.00021728716,0.0026605534],"category_scores_gemma":[0.0010234573,0.00026319866,0.00029907667,0.00050762447,0.00017660229,0.00042821091,0.00079304224,0.00040575687,0.0011531266],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019085473,0.00005782089,0.95493335,0.000030247927,0.000057649926,0.00011691051,0.00014227255,0.0010801114,0.024192832,0.00033450683,0.0009140837,0.017949326],"study_design_scores_gemma":[0.000011411446,0.000065099855,0.9929565,0.000009754782,0.000030637504,0.00008925215,0.00013088812,0.0018891005,0.0018724297,0.00039309374,0.0025417197,0.000009941989],"about_ca_topic_score_codex":0.0028771563,"about_ca_topic_score_gemma":0.0065557193,"teacher_disagreement_score":0.0028771563,"about_ca_system_score_codex":0.00012870756,"about_ca_system_score_gemma":0.000100298625,"threshold_uncertainty_score":0.008900404},"labels":[],"label_agreement":null},{"id":"W3111544325","doi":"10.3847/1538-4357/abd108","title":"Thermal and Turbulent Properties of the Warm Neutral Medium in the Solar Neighborhood","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Agence Nationale de la Recherche","keywords":"Turbulence; Thermal; Radiative transfer; Radiative cooling; Mach number; Condensation; Volume (thermodynamics); Flow (mathematics); Mean kinetic temperature","score_opus":0.01213659448436916,"score_gpt":0.21077938711255237,"score_spread":0.1986427926281832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111544325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99941325,0.00003817787,0.000084865525,0.000008111625,0.0000010681537,0.0000012344823,0.000111284375,0.0000051630545,0.00033687562],"genre_scores_gemma":[0.99967146,0.00001985008,0.000069319205,0.0000023783716,0.0000024716321,0.0000011251564,0.00017980444,0.0000027927567,0.00005087924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994946,0.0000064141586,0.000002357145,0.000015381705,0.00001098233,0.00001545272],"domain_scores_gemma":[0.9998294,0.00004060308,0.000044316916,0.000012590596,0.000025684962,0.000047410766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011241715,0.000112227994,0.0002096243,0.0005761552,0.0002935891,0.00054499006,0.00016714961,0.00013561787,0.00064689806],"category_scores_gemma":[0.00045563784,0.00010867233,0.00012585489,0.0003792493,0.00023406172,0.00029840393,0.00035114726,0.00015552551,0.00009104526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003316293,0.00007397894,0.9181419,0.000035812995,0.00011499307,0.00045860832,0.0006408724,0.00789129,0.06338946,0.0011595738,0.00036342657,0.0073985434],"study_design_scores_gemma":[0.000006748059,0.000023275308,0.9901839,0.0000035636092,0.000014678882,0.000052685544,0.00024471642,0.007654258,0.0013005551,0.00016270812,0.0003435565,0.000009275441],"about_ca_topic_score_codex":0.009473064,"about_ca_topic_score_gemma":0.01094737,"teacher_disagreement_score":0.009473064,"about_ca_system_score_codex":0.00027317888,"about_ca_system_score_gemma":0.00008165236,"threshold_uncertainty_score":0.018835843},"labels":[],"label_agreement":null},{"id":"W3111631962","doi":"10.3847/1538-4357/abccc9","title":"Erratum: “The Red Supergiant Binary Fraction of the Large Magellanic Cloud” (2020, ApJ, 900, 118)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Supergiant; Large Magellanic Cloud; Astrophysics; Astronomy; Binary number; Stars","score_opus":0.010064380580826551,"score_gpt":0.25199794689917593,"score_spread":0.2419335663183494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111631962","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00076873944,0.002968091,0.00029051074,0.040471382,0.9085885,0.000029825618,0.010064493,0.0004500617,0.036368363],"genre_scores_gemma":[0.010876075,0.007688084,0.002643591,0.063856,0.15985925,0.0001627524,0.021223746,0.0013485688,0.73234195],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9992718,0.0000674693,0.00011960878,0.000119846976,0.0003477611,0.00007353151],"domain_scores_gemma":[0.99526453,0.0005752548,0.00029638756,0.00026425818,0.0031349657,0.00046457775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010537981,0.0016320017,0.00096682325,0.003029269,0.0030126844,0.0034020047,0.0012792393,0.0028854953,0.061185256],"category_scores_gemma":[0.008523653,0.00061525044,0.0007716064,0.0018052815,0.0008004263,0.0021407625,0.0011155662,0.0045087696,0.07010334],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000021798161,0.000004248921,0.00009524024,0.000028148292,0.0000017079649,0.000042509946,0.000004035097,0.00001345946,0.000034146105,0.0002994866,0.99682707,0.0026281918],"study_design_scores_gemma":[0.00002087789,0.000019568532,0.0035514436,0.00013820759,0.000013517019,0.00020236056,0.000065739856,0.000086671396,0.0002699483,0.0010282539,0.994582,0.000021436375],"about_ca_topic_score_codex":0.034657247,"about_ca_topic_score_gemma":0.03988996,"teacher_disagreement_score":0.061185256,"about_ca_system_score_codex":0.002387627,"about_ca_system_score_gemma":0.0038370905,"threshold_uncertainty_score":0.20468509},"labels":[],"label_agreement":null},{"id":"W3111673839","doi":"10.3847/1538-4357/abe040","title":"Hubble Space Telescope Observations of Two Faint Dwarf Satellites of Nearby LMC Analogs from MADCASH*","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Space Telescope Science Institute","keywords":"Dwarf galaxy; Local Group; Red-giant branch; Large Magellanic Cloud; Hubble space telescope; Galaxy; Irregular galaxy; Halo; Milky Way","score_opus":0.015127086816456541,"score_gpt":0.22985492222764167,"score_spread":0.21472783541118512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111673839","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983259,0.00002962807,0.000027895629,0.000013818323,0.0000016893974,0.000003034895,0.00043785467,0.00001533311,0.0011449124],"genre_scores_gemma":[0.9984364,0.00001866327,0.000170162,0.000016779051,0.0000047244826,0.000003367364,0.0009862066,0.000005172905,0.0003583247],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999641,0.0000015145282,0.0000012083384,0.000011318498,0.00001036287,0.000011427],"domain_scores_gemma":[0.9998318,0.000009881355,0.000036441463,0.000018228231,0.000019432779,0.000084138715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000054398715,0.00013733578,0.00012690235,0.00061178557,0.00041633134,0.00032699798,0.00019423963,0.00014384848,0.001216227],"category_scores_gemma":[0.00016049945,0.000079259706,0.00007684398,0.00045962518,0.00018816379,0.00014312673,0.0003457186,0.00017337015,0.00023564843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003065758,0.0000936382,0.8945133,0.00004325261,0.00005934798,0.0010170677,0.0013476355,0.0005783196,0.07962277,0.00032960897,0.0022800916,0.019808384],"study_design_scores_gemma":[0.0000072823927,0.000019023284,0.9971264,0.0000025685595,0.000005987363,0.00008847378,0.00013888528,0.00021656934,0.000959743,0.000018763036,0.0014133352,0.000003014189],"about_ca_topic_score_codex":0.03392831,"about_ca_topic_score_gemma":0.08190774,"teacher_disagreement_score":0.03392831,"about_ca_system_score_codex":0.0006210861,"about_ca_system_score_gemma":0.00019275279,"threshold_uncertainty_score":0.06746167},"labels":[],"label_agreement":null},{"id":"W3111856839","doi":"10.3847/1538-4357/ac1da6","title":"First Discovery of New Pulsars and RRATs with CHIME/FRB","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; McGill University; University of British Columbia","funders":"","keywords":"Pulsar; Fast radio burst; Radio astronomy; Active galactic nucleus; Radio telescope; Neutron star","score_opus":0.010199068697154024,"score_gpt":0.2824201574426169,"score_spread":0.27222108874546286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3111856839","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.988913,0.0012070269,0.0027584967,0.0002597692,0.000046211087,0.000038157956,0.00083636463,0.00010997664,0.0058309287],"genre_scores_gemma":[0.9950919,0.00025864207,0.0026596875,0.00010664368,0.00003710603,0.000010028079,0.0010091523,0.00002087087,0.00080596743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996809,0.000013910179,0.00001127321,0.00008084635,0.0001309879,0.000082082384],"domain_scores_gemma":[0.9989496,0.00013408276,0.00030397638,0.00014844214,0.00024280687,0.00022112118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040550227,0.00032950306,0.0003800932,0.0015895118,0.0011802253,0.0012576878,0.00067026523,0.00065276056,0.0016014812],"category_scores_gemma":[0.0013584523,0.00028925325,0.00022294525,0.0014799514,0.00080170226,0.00028027082,0.001033753,0.000714061,0.00030183746],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079475547,0.00011175087,0.82964206,0.0001745658,0.00028322183,0.004317971,0.0013304142,0.0005089824,0.076245464,0.0024382635,0.0028397194,0.08131283],"study_design_scores_gemma":[0.000029145875,0.00010352887,0.9775444,0.000030505867,0.0000592646,0.0015666563,0.00022915148,0.0006710949,0.007832095,0.000337775,0.011561956,0.000034464614],"about_ca_topic_score_codex":0.07178304,"about_ca_topic_score_gemma":0.11335131,"teacher_disagreement_score":0.07178304,"about_ca_system_score_codex":0.0016030357,"about_ca_system_score_gemma":0.0009596756,"threshold_uncertainty_score":0.14273041},"labels":[],"label_agreement":null},{"id":"W3112057487","doi":"10.3847/1538-4357/abd183","title":"On the Use of Field RR Lyrae as Galactic Probes. II. A New ΔS Calibration to Estimate Their Metallicity*","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Astronomical Observatory of Japan; Istituto Nazionale di Astrofisica; Carnegie Institution of Washington","keywords":"Balmer series; Spectral line; RR Lyrae variable; Metallicity; Calibration; Line (geometry); Field (mathematics)","score_opus":0.027812969820915363,"score_gpt":0.25506627167263407,"score_spread":0.22725330185171871,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3112057487","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9468004,0.00052230083,0.04792554,0.000046547506,0.000010457635,0.000050750965,0.00067807036,0.00037512477,0.0035908069],"genre_scores_gemma":[0.9554469,0.00018919937,0.04258499,0.000048851034,0.000019508005,0.00005592558,0.0007371188,0.00005516907,0.00086248625],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990182,0.0003202576,0.000048102112,0.00037066903,0.00019369165,0.000049056358],"domain_scores_gemma":[0.9980654,0.00048391015,0.00044758854,0.0005798372,0.00034474174,0.000078502526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019516718,0.00052024075,0.00021798773,0.0024462522,0.00019890052,0.0005596149,0.0006024075,0.00023098764,0.0009776601],"category_scores_gemma":[0.0024453574,0.000208689,0.00021617602,0.00085332134,0.00039581262,0.00056441565,0.0007373017,0.0002576603,0.0006010056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022500621,0.00007388248,0.73132694,0.00010700874,0.000111114015,0.00006295383,0.0002828947,0.005158154,0.050443962,0.0011002817,0.0005669723,0.21054082],"study_design_scores_gemma":[0.000052777068,0.00029579306,0.9049339,0.000043219243,0.00008255624,0.0004149639,0.0002454372,0.03987592,0.043862753,0.0012961348,0.008857343,0.000039229042],"about_ca_topic_score_codex":0.0024203565,"about_ca_topic_score_gemma":0.0041703475,"teacher_disagreement_score":0.0024462522,"about_ca_system_score_codex":0.00039144538,"about_ca_system_score_gemma":0.0001374343,"threshold_uncertainty_score":0.010321498},"labels":[],"label_agreement":null},{"id":"W3112193767","doi":"10.3847/1538-4357/abe123","title":"Follow-up of Astrophysical Transients in Real Time with the IceCube Neutrino Observatory","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Snolab","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Observatory; Neutrino; Cosmic ray; Pipeline (software); Neutrino detector; COSMIC cancer database; Cosmic background radiation","score_opus":0.010172907753492203,"score_gpt":0.2119243779953804,"score_spread":0.2017514702418882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3112193767","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7066172,0.0017893683,0.05713595,0.0021400684,0.0006682741,0.00070076255,0.1335625,0.01327673,0.08410925],"genre_scores_gemma":[0.7689305,0.0006659543,0.108526394,0.0006715418,0.00024076842,0.0004001711,0.1083391,0.0023270263,0.009898481],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99907196,0.00011720681,0.000039335966,0.00022918431,0.00037999786,0.00016229175],"domain_scores_gemma":[0.9974611,0.0003909122,0.00046150942,0.00041116885,0.00096480723,0.0003105738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020060646,0.00053613354,0.0003985015,0.0022725672,0.00070005096,0.0013920339,0.00049199193,0.00037991005,0.005050549],"category_scores_gemma":[0.00382474,0.00032402168,0.0005252571,0.0021539961,0.0002478737,0.0008559434,0.0015760453,0.0009168931,0.0025933625],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001309673,0.00022592103,0.7419018,0.00028482554,0.0005853869,0.0007870296,0.0008257027,0.0059926156,0.048387572,0.0033168858,0.08063296,0.115749545],"study_design_scores_gemma":[0.00020113852,0.0001904207,0.7645215,0.00015365306,0.00027430215,0.00044959688,0.0006774702,0.019643135,0.029160343,0.0042283335,0.18034716,0.00015294706],"about_ca_topic_score_codex":0.017961314,"about_ca_topic_score_gemma":0.042941194,"teacher_disagreement_score":0.017961314,"about_ca_system_score_codex":0.00067346904,"about_ca_system_score_gemma":0.0011527939,"threshold_uncertainty_score":0.035713553},"labels":[],"label_agreement":null},{"id":"W3112478714","doi":"10.3847/1538-4357/abd47f","title":"Observational Evidence for Enhanced Black Hole Accretion in Giant Elliptical Galaxies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Perimeter Institute; University of Waterloo","funders":"National Aeronautics and Space Administration; California Institute of Technology; Princeton University; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Astrophysics; Physics; Galaxy; Accretion (finance); Star formation; Elliptical galaxy; Astronomy","score_opus":0.037271949829518106,"score_gpt":0.2757671336860439,"score_spread":0.2384951838565258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3112478714","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99955183,0.000046217498,0.00004467003,0.000020053738,9.796494e-7,0.0000014314924,0.00008199958,0.0000059064864,0.0002469301],"genre_scores_gemma":[0.99984443,0.000014238644,0.00002559949,0.0000065030554,0.0000036977572,5.7571987e-7,0.000073442556,0.0000010012669,0.000030505335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965847,0.000085259475,0.000026190397,0.000081483435,0.00007072689,0.000077809294],"domain_scores_gemma":[0.9956731,0.00091676146,0.0018811855,0.0004093902,0.0003329857,0.00078653684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006680548,0.00018726512,0.0002823903,0.0013259976,0.00032422435,0.0006368209,0.00032700362,0.00036215413,0.0013186133],"category_scores_gemma":[0.0020234145,0.00019344801,0.00019342736,0.0007096782,0.0007224631,0.00030720487,0.000582647,0.00024446042,0.00033219325],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000032112413,0.0000143408815,0.9974503,0.000004262125,0.000016574588,0.000044739223,0.00009190992,0.000020132056,0.0016910352,0.000029501782,0.000029253388,0.00057590124],"study_design_scores_gemma":[0.0000013831418,0.000017347003,0.9996308,0.000001098048,0.000003645021,0.00008299527,0.00006934574,0.000049424034,0.000088901266,0.000012785622,0.000041476687,7.592128e-7],"about_ca_topic_score_codex":0.0022971893,"about_ca_topic_score_gemma":0.0030140493,"teacher_disagreement_score":0.0022971893,"about_ca_system_score_codex":0.00019065512,"about_ca_system_score_gemma":0.000090572794,"threshold_uncertainty_score":0.0045675635},"labels":[],"label_agreement":null},{"id":"W3112990476","doi":"10.3847/1538-4357/abbfb6","title":"The Sun: Light Dark Matter and Sterile Neutrinos","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Solar neutrino; Neutrino; Neutrino oscillation; Solar neutrino problem; Particle physics; Measurements of neutrino speed; Sterile neutrino; Borexino; Dark matter; Neutrino detector; Astrophysics","score_opus":0.007348044383030514,"score_gpt":0.20470138542519406,"score_spread":0.19735334104216354,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3112990476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97118104,0.0013460821,0.0118821245,0.0011884395,0.00013312869,0.00000703303,0.00009118746,0.00004901778,0.014121942],"genre_scores_gemma":[0.9983392,0.00015744093,0.000805616,0.00007667857,0.00002432594,0.0000017153177,0.000015826612,0.000004049316,0.00057516777],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998029,0.000062898085,0.0000054428324,0.000051426865,0.00004037157,0.00003697027],"domain_scores_gemma":[0.9994185,0.00026259894,0.00013015929,0.00006193308,0.000030519048,0.00009642288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008338621,0.00023228738,0.0003081723,0.00032515422,0.0003890425,0.0016228025,0.00025332175,0.00077279995,0.0019274886],"category_scores_gemma":[0.0010045847,0.000124425,0.00031692602,0.00018318625,0.0012311654,0.0012554078,0.0006648949,0.00040547943,0.00013192871],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000855755,0.00014594838,0.09306863,0.00020124018,0.000118633696,0.001100338,0.00053476554,0.015501292,0.04107198,0.81796044,0.0024658802,0.026975064],"study_design_scores_gemma":[0.0001829929,0.0002508258,0.0395667,0.00009457617,0.00008450308,0.0008369732,0.00082457176,0.1180655,0.01283862,0.8173623,0.00981017,0.00008225458],"about_ca_topic_score_codex":0.001209065,"about_ca_topic_score_gemma":0.0010391908,"teacher_disagreement_score":0.0019274886,"about_ca_system_score_codex":0.0003366051,"about_ca_system_score_gemma":0.0002384712,"threshold_uncertainty_score":0.00644809},"labels":[],"label_agreement":null},{"id":"W3113302476","doi":"10.3847/1538-4357/abd0fc","title":"Observations of Magnetic Fields Surrounding LkHα 101 Taken by the BISTRO Survey with JCMT-POL-2","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; McMaster University; Queen's University; University of Manitoba; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec; Herzberg Institute of Astrophysics","funders":"Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; Seoul National University; Academia Sinica; Science and Technology Facilities Council; National Research Foundation; National Foundation for Science and Technology Development; Chinese Academy of Sciences; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Magnetic field; Polarization (electrochemistry); Redshift; Radiative transfer; James Clerk Maxwell Telescope; Spectral index; Star formation; Polarimetry; Molecular cloud","score_opus":0.028186141255539456,"score_gpt":0.24463316622246098,"score_spread":0.21644702496692153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3113302476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948368,0.0001033851,0.00039728207,0.000029468234,0.0000085205065,0.000021356136,0.0010570844,0.00008117219,0.0034649575],"genre_scores_gemma":[0.9970892,0.00004361338,0.00084733975,0.000028613322,0.000016703936,0.000008882594,0.0016231519,0.000010473781,0.0003320978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998167,0.00001530227,0.00000767338,0.000046040157,0.00007547831,0.000038920218],"domain_scores_gemma":[0.999419,0.000033065313,0.00017956115,0.00008313428,0.000098994606,0.00018627207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019109466,0.00021451167,0.00021693173,0.00080564705,0.0003751749,0.0005039186,0.000347723,0.00021904404,0.000813546],"category_scores_gemma":[0.00038933932,0.00015951142,0.000106882784,0.00045773658,0.00023430688,0.00020670766,0.00044366042,0.0002665094,0.00030841393],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042058533,0.000121602665,0.8377117,0.00006579683,0.00010423639,0.0007029508,0.0003891838,0.0009865431,0.14116994,0.00021827508,0.0014844786,0.0166248],"study_design_scores_gemma":[0.000025122547,0.000043637443,0.9941707,0.000008114659,0.000015712803,0.00021301526,0.000068928835,0.0010595468,0.0026678904,0.000018413171,0.001703221,0.0000056485396],"about_ca_topic_score_codex":0.009925176,"about_ca_topic_score_gemma":0.027979806,"teacher_disagreement_score":0.009925176,"about_ca_system_score_codex":0.00042359333,"about_ca_system_score_gemma":0.0002905329,"threshold_uncertainty_score":0.01973486},"labels":[],"label_agreement":null},{"id":"W3113370962","doi":"10.3847/1538-4357/abd1d5","title":"Discovery of a Damped Lyα Galaxy at z ∼ 3 toward the Quasar SDSS J011852+040644","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Ministério da Ciência, Tecnologia e Inovação; China Postdoctoral Science Foundation; Smithsonian Institution; U.S. Department of Energy; Fondazione Cariplo; National Natural Science Foundation of China; Agence Nationale de la Recherche; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; European Commission; California Institute of Technology; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University","keywords":"Quasar; Galaxy; Redshift; Luminosity; Star formation; Spectral line; Impact parameter; Line (geometry)","score_opus":0.010989577027848134,"score_gpt":0.2200652591056597,"score_spread":0.20907568207781155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3113370962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998086,0.000056588644,0.000528412,0.000031989086,0.000004877881,0.000007235282,0.0002343504,0.00009630892,0.000954252],"genre_scores_gemma":[0.9987324,0.00001709172,0.0005174458,0.000036215377,0.000005855025,0.000003408074,0.00032243252,0.0000048076536,0.00036042897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998665,0.000010667742,0.0000072956664,0.000037663714,0.000043668257,0.00003426149],"domain_scores_gemma":[0.999622,0.000028809402,0.000114856455,0.000038850307,0.000046501627,0.00014901099],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026573552,0.00018948907,0.00018938433,0.00088094024,0.00031717448,0.0005493129,0.00027598944,0.00026457413,0.0019425434],"category_scores_gemma":[0.00040027953,0.00018220046,0.0001784531,0.00035514074,0.0002132213,0.00014987527,0.00047846464,0.00024766862,0.00054457725],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015954692,0.00008901108,0.8969699,0.000031780553,0.00005893645,0.0009852535,0.00033302003,0.0002327823,0.090578,0.0002792333,0.0008085452,0.009473975],"study_design_scores_gemma":[0.000009370197,0.00009707843,0.99302155,0.0000047156946,0.000018364459,0.0007604677,0.00008516009,0.000858916,0.0035659713,0.000063736545,0.0015076164,0.0000071070135],"about_ca_topic_score_codex":0.002269987,"about_ca_topic_score_gemma":0.002790026,"teacher_disagreement_score":0.002269987,"about_ca_system_score_codex":0.00022491654,"about_ca_system_score_gemma":0.000086894,"threshold_uncertainty_score":0.006498456},"labels":[],"label_agreement":null},{"id":"W3115202110","doi":"10.3847/1538-4357/abfe6d","title":"The Atacama Cosmology Telescope: Detection of Millimeter-wave Transient Sources","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; University of Toronto; Science and Technology Facilities Council; European Commission; Flatiron Health; Government of Ontario; Compute Canada; University of Pennsylvania; Princeton University; Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Spectral index; Flux (metallurgy); Cosmology; Transient (computer programming); Spectral line","score_opus":0.00961028028865882,"score_gpt":0.2081117156103706,"score_spread":0.19850143532171177,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3115202110","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9839828,0.00066392386,0.0028936982,0.0002896886,0.000047161513,0.00005183652,0.0016824474,0.00023206847,0.010156402],"genre_scores_gemma":[0.9933248,0.00014876568,0.002765993,0.00012516556,0.000052940646,0.000019944247,0.0023025125,0.0000303936,0.0012295916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996972,0.000025537689,0.0000143860225,0.000078495184,0.0001271192,0.00005718603],"domain_scores_gemma":[0.9988732,0.00012214147,0.00038496708,0.00018235685,0.0001898741,0.00024743902],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007166481,0.0002305995,0.00023652361,0.0012470376,0.0008454299,0.00088531297,0.00052321533,0.0006168705,0.0013844656],"category_scores_gemma":[0.00055538013,0.00023543596,0.0002884161,0.0013400293,0.00031545645,0.0003289607,0.00054316333,0.0006677999,0.0005903356],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004916417,0.00017653938,0.82565796,0.00016435393,0.0001823088,0.0015777353,0.0011821488,0.0005293758,0.120639876,0.0010986369,0.0051612547,0.043138184],"study_design_scores_gemma":[0.000018861476,0.000071235845,0.99133307,0.00001054632,0.000023730623,0.00043770892,0.00011584175,0.0005274867,0.0037169082,0.00009433887,0.0036364668,0.000013707171],"about_ca_topic_score_codex":0.006816772,"about_ca_topic_score_gemma":0.011742741,"teacher_disagreement_score":0.006816772,"about_ca_system_score_codex":0.000631054,"about_ca_system_score_gemma":0.00037981773,"threshold_uncertainty_score":0.013554215},"labels":[],"label_agreement":null},{"id":"W3116194887","doi":"10.3847/1538-4357/abee78","title":"A Deep Chandra X-Ray Observatory Study of the Millisecond Pulsar Population in the Globular Cluster Terzan 5","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Globular cluster; Millisecond pulsar; Observatory; Pulsar; Population; Neutron star; Millisecond; Cluster (spacecraft); Star cluster","score_opus":0.01437490831003789,"score_gpt":0.23505977653234722,"score_spread":0.22068486822230932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3116194887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99956125,0.000033350443,0.000025982023,0.0000045777965,0.0000010312441,0.0000017559311,0.00016571558,0.0000016908234,0.00020464684],"genre_scores_gemma":[0.9986878,0.000051501756,0.00013526334,0.000005388088,0.0000037840798,0.0000026802354,0.0008877248,0.0000019014669,0.00022391556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999238,0.000006325759,0.000004458868,0.00002205575,0.000017101765,0.000026280024],"domain_scores_gemma":[0.99968433,0.000025622254,0.00014309549,0.00003162801,0.00004205455,0.0000732074],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017260415,0.00013592314,0.00015313455,0.0012575794,0.0002405846,0.00036749442,0.00018142762,0.00010940484,0.00048379996],"category_scores_gemma":[0.00039293492,0.0000803523,0.00016004831,0.00081696815,0.00013791346,0.00021417529,0.00050544884,0.00016969028,0.00014257534],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020477339,0.00003851374,0.9777475,0.000017671155,0.000044582783,0.00032634466,0.00033552197,0.00046520992,0.013084565,0.0001318275,0.0002278442,0.0073756115],"study_design_scores_gemma":[0.0000018714852,0.000014973018,0.99921715,0.0000015316614,0.0000031508798,0.00008189422,0.000054821016,0.00017370006,0.00015976946,0.000009620942,0.0002801999,0.0000013784263],"about_ca_topic_score_codex":0.007619183,"about_ca_topic_score_gemma":0.012459224,"teacher_disagreement_score":0.007619183,"about_ca_system_score_codex":0.00032016702,"about_ca_system_score_gemma":0.00019992214,"threshold_uncertainty_score":0.015149653},"labels":[],"label_agreement":null},{"id":"W3116624562","doi":"10.3847/1538-4357/abd558","title":"Absolute Calibration of Diffuse Radio Surveys at 45 and 150 MHz","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Cosmic microwave background; Calibration; Sigma; Sky; Brightness temperature; Astrophysics; Scale (ratio); Range (aeronautics); Remote sensing; Brightness; Astronomy; Optics; Geography","score_opus":0.011200127608475607,"score_gpt":0.2166854672437171,"score_spread":0.2054853396352415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3116624562","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95345473,0.00071513595,0.030923333,0.00010084422,0.000037439724,0.000020359663,0.0018700708,0.0005917473,0.012286437],"genre_scores_gemma":[0.9897674,0.00011258321,0.007879002,0.00005641503,0.000013369224,0.000019793115,0.0016242912,0.00006573142,0.0004614362],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99896824,0.00022357788,0.0000403906,0.00039442262,0.0002726937,0.00010063596],"domain_scores_gemma":[0.99834394,0.00026473525,0.00042919992,0.00046580902,0.00038994738,0.00010630456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012148208,0.00029778492,0.00025763645,0.0010554706,0.00018181968,0.0005438443,0.0005617946,0.0003201032,0.000996376],"category_scores_gemma":[0.0032484792,0.00025486495,0.00023938266,0.0008727663,0.00027219925,0.0005695324,0.0007665915,0.0003494319,0.00059553445],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003884767,0.000053273026,0.7983666,0.00010555939,0.00022677114,0.00006736384,0.0005362934,0.01244727,0.07387497,0.0037565816,0.0026090012,0.10756785],"study_design_scores_gemma":[0.000023795365,0.000051874023,0.9728757,0.00002415944,0.000054565877,0.000104508166,0.000091768925,0.0066623073,0.012802594,0.0006664038,0.006610886,0.00003150366],"about_ca_topic_score_codex":0.0055263476,"about_ca_topic_score_gemma":0.009481404,"teacher_disagreement_score":0.0055263476,"about_ca_system_score_codex":0.00056474574,"about_ca_system_score_gemma":0.00017208779,"threshold_uncertainty_score":0.010988355},"labels":[],"label_agreement":null},{"id":"W3117367066","doi":"10.3847/1538-4357/abdf48","title":"RR Lyrae Variables in Messier 53: Near-infrared Period–Luminosity Relations and the Calibration Using Gaia Early Data Release 3","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"RR Lyrae variable; Globular cluster; Cepheid variable; Parallax; Variable star; Stars; Homogeneous; Calibration","score_opus":0.01822220019376431,"score_gpt":0.23224928414261103,"score_spread":0.21402708394884673,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3117367066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98528844,0.0006330147,0.0018460876,0.00010565561,0.000012019912,0.000037921094,0.0056191403,0.00044220535,0.0060155066],"genre_scores_gemma":[0.989677,0.0001810756,0.0022888898,0.000058432157,0.000023624447,0.00004226904,0.006450516,0.00009260748,0.0011856877],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997787,0.00002248173,0.000015520967,0.0001014873,0.000041912135,0.000039895694],"domain_scores_gemma":[0.9994568,0.0000615151,0.00024404406,0.000116114265,0.0000631141,0.000058429923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004270825,0.0003183326,0.00030273027,0.0017209994,0.00022140163,0.0005840943,0.00031920816,0.00016220473,0.0023100213],"category_scores_gemma":[0.0009340985,0.00011867793,0.00029736164,0.0010346954,0.00020762935,0.00025562252,0.00047502088,0.00023088044,0.0013843951],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037750014,0.00002094945,0.92003274,0.000082210325,0.00014324792,0.00025280795,0.0007150793,0.0029849694,0.014871333,0.0009800184,0.0059508537,0.053588286],"study_design_scores_gemma":[0.000008473263,0.000012852984,0.9938921,0.000009641535,0.000015420432,0.000032736745,0.000042480002,0.000873238,0.0009242814,0.00005818806,0.0041246936,0.0000058030087],"about_ca_topic_score_codex":0.052416015,"about_ca_topic_score_gemma":0.07386734,"teacher_disagreement_score":0.052416015,"about_ca_system_score_codex":0.00096005417,"about_ca_system_score_gemma":0.00014518306,"threshold_uncertainty_score":0.10422188},"labels":[],"label_agreement":null},{"id":"W3118286995","doi":"10.3847/1538-4357/abe2a7","title":"The Center of Expansion and Age of the Oxygen-rich Supernova Remnant 1E 0102.2-7219","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Supernova remnant; Proper motion; Supernova; Center (category theory); Telescope; Asymmetry; Position (finance); Hubble space telescope","score_opus":0.010296635975283875,"score_gpt":0.22248384003509472,"score_spread":0.21218720405981084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118286995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978404,0.00014390388,0.0004472308,0.000009712201,0.000004522373,0.000003638038,0.000416173,0.000025883277,0.0011084998],"genre_scores_gemma":[0.99822766,0.00005954416,0.00042914134,0.000005721008,0.000005412039,0.000003258265,0.0010364699,0.000009211476,0.00022371062],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999038,0.000008452403,0.000006393084,0.000033444827,0.00002959331,0.000018331302],"domain_scores_gemma":[0.99949515,0.000059206708,0.00021436512,0.000046228848,0.00009721105,0.00008777614],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045326306,0.00023150271,0.00018535135,0.0009210466,0.00020861758,0.00048058416,0.0002923866,0.00020085588,0.0007580413],"category_scores_gemma":[0.0005756521,0.0001386902,0.00019841487,0.0003421217,0.00013972851,0.00025786206,0.00031966012,0.00018624228,0.00033734526],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022397912,0.000032121785,0.9499598,0.00002100958,0.000049858674,0.00018797025,0.0001010337,0.0010679394,0.042542346,0.0001605824,0.00027740758,0.0053758966],"study_design_scores_gemma":[0.0000030493366,0.000024997416,0.99715436,0.0000033354497,0.0000067794836,0.00013939927,0.000031175186,0.00063334877,0.0015304292,0.00001841084,0.00044968346,0.0000051650804],"about_ca_topic_score_codex":0.0045754104,"about_ca_topic_score_gemma":0.0051913774,"teacher_disagreement_score":0.0045754104,"about_ca_system_score_codex":0.00035286054,"about_ca_system_score_gemma":0.000085661144,"threshold_uncertainty_score":0.009097517},"labels":[],"label_agreement":null},{"id":"W3118314862","doi":"10.3847/1538-4357/abd946","title":"Ultrafaint [C ii] Emission in a Redshift = 2 Gravitationally Lensed Metal-poor Dwarf Galaxy","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Institutes of Natural Sciences; National Astronomical Observatory of Japan; Comisión Nacional de Investigación Científica y Tecnológica; ARC Centre of Excellence for All-Sky Astrophysics; Centre National de la Recherche Scientifique; Canadian Space Agency; Max-Planck-Gesellschaft; Leids Kerkhoven-Bosscha Fonds; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Reionization; Redshift; Galaxy; Metallicity; Line (geometry); Emission spectrum; Dwarf galaxy","score_opus":0.011576967619423027,"score_gpt":0.24761434589437753,"score_spread":0.2360373782749545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118314862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99956125,0.0000139059275,0.00007365214,0.0000070659303,4.5294652e-7,0.0000011944836,0.00005724853,0.00001655918,0.00026858997],"genre_scores_gemma":[0.9996282,0.000006870359,0.00012450044,0.000007726445,0.0000016317706,9.764166e-7,0.00013829496,0.0000024607114,0.00008931991],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999565,0.0000036965107,0.0000015699461,0.000014073746,0.0000073131887,0.000016965803],"domain_scores_gemma":[0.99982387,0.000014217183,0.000053494306,0.000013649889,0.000013862795,0.0000809492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008773921,0.0002554471,0.00018006045,0.00049897685,0.00020297515,0.00034542044,0.00019578593,0.00018227343,0.0007657723],"category_scores_gemma":[0.00013329882,0.00013064255,0.00014068454,0.0002553962,0.00016272042,0.00011211248,0.00027180894,0.00014075446,0.00013896383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038275457,0.00012444961,0.8218122,0.000023845743,0.00007794752,0.001016946,0.00028421305,0.0013590318,0.16839144,0.00038910517,0.00042416877,0.0057138414],"study_design_scores_gemma":[0.000010855692,0.000064990265,0.9940692,0.0000020500916,0.000014633881,0.00021394157,0.00007463119,0.0023201413,0.0027481818,0.00007910858,0.00039789994,0.000004312779],"about_ca_topic_score_codex":0.0069287387,"about_ca_topic_score_gemma":0.008908183,"teacher_disagreement_score":0.0069287387,"about_ca_system_score_codex":0.0003463226,"about_ca_system_score_gemma":0.00007307825,"threshold_uncertainty_score":0.013776839},"labels":[],"label_agreement":null},{"id":"W3118361769","doi":"10.3847/1538-4357/abddbb","title":"VLA Resolves Unexpected Radio Structures in the Perseus Cluster of Galaxies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"National Astronomical Observatory of Japan; Gates Cambridge Trust; Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada; Science and Technology Facilities Council; National Radio Astronomy Observatory","keywords":"Galaxy cluster; Radio galaxy; Jansky; Brightest cluster galaxy; X-shaped radio galaxy; Galaxy; Intracluster medium; Interacting galaxy; Cluster (spacecraft)","score_opus":0.007497365485705193,"score_gpt":0.21640530699862037,"score_spread":0.20890794151291517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118361769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981812,0.00008438811,0.00031630986,0.000026031585,0.0000038046626,0.0000025596603,0.00022897715,0.000063906795,0.0010927259],"genre_scores_gemma":[0.99886405,0.000016817548,0.00047787107,0.00001658014,0.0000066357024,0.0000024589076,0.00034809037,0.0000069801495,0.00026041805],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.0000052336054,0.0000015687332,0.00002385691,0.000014208219,0.00001828088],"domain_scores_gemma":[0.9997923,0.000022654258,0.00005128067,0.000038274204,0.00002759676,0.0000678909],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014995274,0.00022331286,0.00016278561,0.000923569,0.00022714447,0.0004015905,0.00021997269,0.0001597187,0.0008211276],"category_scores_gemma":[0.00026010608,0.00014289682,0.000083611405,0.00039950683,0.00020559729,0.00014175805,0.0004455519,0.00014741054,0.00027187789],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031051246,0.00005752773,0.8151131,0.000052388983,0.00011116692,0.0011441427,0.0011049255,0.0018163796,0.1399456,0.00092311477,0.003082455,0.036338586],"study_design_scores_gemma":[0.00001135826,0.00002496846,0.9949787,0.0000043321943,0.000008709743,0.00020911619,0.00023174661,0.00095227384,0.0016977631,0.00016606074,0.0017099833,0.0000049433147],"about_ca_topic_score_codex":0.0032754242,"about_ca_topic_score_gemma":0.007126562,"teacher_disagreement_score":0.0032754242,"about_ca_system_score_codex":0.00028915948,"about_ca_system_score_gemma":0.00010675779,"threshold_uncertainty_score":0.0065127015},"labels":[],"label_agreement":null},{"id":"W3118410088","doi":"10.3847/1538-4357/abdab3","title":"Eruptive Behavior of Magnetically Layered Protoplanetary Disks in Low-metallicity Environments","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"European Research Council; Austrian Science Fund","keywords":"Metallicity; Astrophysics; Physics; Accretion (finance); Protoplanetary disk; Protostar; Star formation; Opacity; Stars; Astronomy","score_opus":0.009348914000289494,"score_gpt":0.2327983239222502,"score_spread":0.2234494099219607,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118410088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999572,0.00002222969,0.00013592839,0.000009868279,8.916348e-7,0.0000016077967,0.000035252422,0.00001159523,0.00021065694],"genre_scores_gemma":[0.9997334,0.000014128182,0.00013020005,0.0000039700117,7.1967094e-7,0.000001486089,0.000049371116,0.0000035146368,0.000063199215],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995375,0.000007932868,0.0000033825474,0.000011350745,0.000006706392,0.000016921029],"domain_scores_gemma":[0.9996755,0.000106836065,0.00007456823,0.000022671322,0.00003520406,0.00008524751],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012934931,0.0002733357,0.00026768385,0.00039948453,0.00040898848,0.0006319155,0.0004731317,0.0003795676,0.0007560376],"category_scores_gemma":[0.000818385,0.00020210457,0.00026799232,0.00022035556,0.00039828615,0.0003416644,0.00054115907,0.00025885054,0.0000974214],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000561431,0.00025005112,0.35618895,0.0001034956,0.00020575002,0.0014100209,0.0007072627,0.55928797,0.074704535,0.0015942623,0.0003495801,0.004636655],"study_design_scores_gemma":[0.00011143042,0.00034143458,0.16934747,0.000023500865,0.00007521159,0.0002556659,0.000587791,0.81990045,0.008053109,0.00072306936,0.0005382986,0.000042556967],"about_ca_topic_score_codex":0.004625264,"about_ca_topic_score_gemma":0.002445753,"teacher_disagreement_score":0.004625264,"about_ca_system_score_codex":0.00055567984,"about_ca_system_score_gemma":0.00016824255,"threshold_uncertainty_score":0.009196699},"labels":[],"label_agreement":null},{"id":"W3118558754","doi":"10.3847/1538-4357/ac0058","title":"mirkwood: Fast and Accurate SED Modeling Using Machine Learning","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"University of Toronto; City University of New York; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; sed; Astrophysics; Astronomy; Medicine","score_opus":0.015943482951587148,"score_gpt":0.23317999949261875,"score_spread":0.2172365165410316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118558754","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.027725274,0.00018910907,0.8693259,0.00025250047,0.00014107102,0.000099856305,0.0028216925,0.09763344,0.0018111849],"genre_scores_gemma":[0.2723729,0.00016211234,0.70457864,0.00027351317,0.000073735326,0.00025664357,0.007982315,0.011983261,0.0023169843],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994411,0.00012064989,0.000035082303,0.00013948463,0.00021493816,0.000048804504],"domain_scores_gemma":[0.99799347,0.00074173446,0.0002019529,0.0005315065,0.00038092362,0.0001503722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019216676,0.0013404335,0.0010117264,0.0014862261,0.0008303975,0.001546357,0.0042823725,0.0012566,0.0049688513],"category_scores_gemma":[0.0077419057,0.0011248672,0.00152866,0.0009412554,0.00047176558,0.0025021369,0.0019174708,0.002300188,0.0032106463],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020333802,0.00024143555,0.012839287,0.00023996369,0.00043099234,0.00029057672,0.0002498468,0.79811853,0.008828163,0.015004639,0.039440714,0.12411254],"study_design_scores_gemma":[0.00000961216,0.0000061042406,0.0003164677,0.000006543263,0.0000045402726,0.000019342984,0.0000073408514,0.99234116,0.0012630892,0.0038235101,0.0021873037,0.0000149418265],"about_ca_topic_score_codex":0.009613319,"about_ca_topic_score_gemma":0.011334971,"teacher_disagreement_score":0.009613319,"about_ca_system_score_codex":0.0010602887,"about_ca_system_score_gemma":0.0014670513,"threshold_uncertainty_score":0.019114673},"labels":[],"label_agreement":null},{"id":"W3118971036","doi":"10.3847/1538-4357/abd71e","title":"SITELLE Hα Imaging Spectroscopy of z ∼ 0.25 Clusters: Emission-line Galaxy Detection and Ionized Gas Offset in Abell 2390 and Abell 2465","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"York University; Université de Montréal; Centre for Research in Astrophysics of Québec; Université Laval; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Galaxy; Ram pressure; Galaxy cluster; Virial theorem; Halo; Spectrograph; Integral field spectrograph; Star formation; Cluster (spacecraft); Radio galaxy","score_opus":0.005441166055791095,"score_gpt":0.21619185434372293,"score_spread":0.21075068828793184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3118971036","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99852115,0.000027323333,0.00011957925,0.000014456765,0.0000011754616,0.000004518631,0.0005491329,0.000039393093,0.00072328135],"genre_scores_gemma":[0.9969856,0.000018216637,0.000820784,0.000017499013,0.000005671154,0.0000071820878,0.0016932966,0.000014373899,0.0004373461],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997377,0.000024095876,0.000009363239,0.00009177624,0.000063720494,0.000073278425],"domain_scores_gemma":[0.99931216,0.00005597427,0.00018766391,0.00006148907,0.00012428564,0.00025852438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042118225,0.00027021806,0.00029111348,0.0017705314,0.00083773833,0.0006120244,0.00043300592,0.00031611125,0.0012231772],"category_scores_gemma":[0.00044301446,0.00026120798,0.00027316532,0.0006988062,0.00021143653,0.0002497218,0.00061778305,0.00022308323,0.00053407525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000514532,0.00017259417,0.9113543,0.000021173892,0.000094343275,0.00036910863,0.0005712327,0.0006266158,0.07877732,0.00015177325,0.0011497103,0.006197267],"study_design_scores_gemma":[0.000009583789,0.000025832294,0.9968071,0.0000032356843,0.000008863057,0.000072081675,0.000105712395,0.0006385276,0.0019538796,0.000011562847,0.0003568115,0.0000067440087],"about_ca_topic_score_codex":0.048229456,"about_ca_topic_score_gemma":0.1407101,"teacher_disagreement_score":0.048229456,"about_ca_system_score_codex":0.0008452567,"about_ca_system_score_gemma":0.00023644062,"threshold_uncertainty_score":0.095897436},"labels":[],"label_agreement":null},{"id":"W3119014998","doi":"10.3847/1538-4357/abe59e","title":"Mass Ejection in Failed Supernovae: Equation of State and Neutrino Loss Dependence","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutrino; Ejecta; Supernova; Equation of state; Type II supernova; Supergiant; Observable; Stellar structure; Stars; Nucleosynthesis","score_opus":0.012886998730090356,"score_gpt":0.23213717296622605,"score_spread":0.2192501742361357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119014998","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949003,0.00006258901,0.0035599007,0.00006124855,0.0000069278026,0.000007342831,0.00013907911,0.00006961915,0.0011931233],"genre_scores_gemma":[0.998998,0.000020679756,0.00063516304,0.000009015665,0.0000017368284,0.0000061783317,0.000094898445,0.000027261947,0.00020712984],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987614,0.000027623457,0.000010291553,0.000017502432,0.000037197668,0.000031242962],"domain_scores_gemma":[0.9984957,0.00086103816,0.00025748578,0.00015360684,0.0001537597,0.00007839501],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006148454,0.00036450615,0.0003381733,0.00024288803,0.00019440195,0.0005224252,0.00065098744,0.00034858615,0.0008594815],"category_scores_gemma":[0.004171205,0.00022682548,0.00044223916,0.00017591726,0.00041630195,0.00043080468,0.00043849615,0.00043213976,0.00012001328],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002626508,0.00009229412,0.1311764,0.000078938145,0.00012043037,0.00057383423,0.000113008784,0.8203262,0.03740665,0.0043124133,0.00036207325,0.005175116],"study_design_scores_gemma":[0.0000133899375,0.00006953146,0.018708557,0.000006477057,0.000014578785,0.0000826712,0.000017230805,0.9717056,0.008471394,0.0007365541,0.00015952336,0.000014455872],"about_ca_topic_score_codex":0.0028983818,"about_ca_topic_score_gemma":0.0014564084,"teacher_disagreement_score":0.0028983818,"about_ca_system_score_codex":0.0005560902,"about_ca_system_score_gemma":0.00022009519,"threshold_uncertainty_score":0.005763054},"labels":[],"label_agreement":null},{"id":"W3119296872","doi":"10.3847/1538-4357/abe1bc","title":"The Clusters Hiding in Plain Sight (CHiPS) Survey: Complete Sample of Extreme BCG Clusters","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Genomic variations and chromosomal abnormalities","field":"Biochemistry, Genetics and Molecular Biology","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Princeton University; Queen's University Belfast; National Aeronautics and Space Administration; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Sample (material); Astronomy; Sight; Astrophysics; Galaxy cluster; Galaxy","score_opus":0.02562239072659478,"score_gpt":0.22871944737535266,"score_spread":0.20309705664875788,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119296872","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99570787,0.000097501215,0.00017117514,0.000014817611,0.000002102055,0.000015604495,0.003149902,0.0000227859,0.0008181919],"genre_scores_gemma":[0.9904585,0.000080086844,0.00036218163,0.000023459086,0.000007971998,0.000015980324,0.008521978,0.000013857278,0.00051580934],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997118,0.000023051702,0.000016231957,0.00010331046,0.000062823055,0.00008284052],"domain_scores_gemma":[0.9988877,0.000067868685,0.00031064716,0.0001967655,0.0001389239,0.00039804683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002945505,0.00019092583,0.00023420034,0.0011596793,0.0003905944,0.00042722278,0.00038514112,0.0001437936,0.0012523523],"category_scores_gemma":[0.0006747668,0.00018335732,0.00014852828,0.0007924817,0.00025944182,0.00026984268,0.0008937133,0.00019767239,0.00063961855],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013368299,0.000034524375,0.98977953,0.00001910833,0.000037451384,0.000056410663,0.00022983427,0.00012332576,0.0034380765,0.000090451846,0.0014004894,0.004657186],"study_design_scores_gemma":[0.000004755888,0.00001605616,0.9990395,0.0000031510106,0.000009405691,0.000048456932,0.00006196029,0.00007583688,0.00014429749,0.0000102419635,0.0005842555,0.0000020470882],"about_ca_topic_score_codex":0.020335207,"about_ca_topic_score_gemma":0.029405095,"teacher_disagreement_score":0.020335207,"about_ca_system_score_codex":0.00022401105,"about_ca_system_score_gemma":0.0003259513,"threshold_uncertainty_score":0.040433645},"labels":[],"label_agreement":null},{"id":"W3119390322","doi":"10.3847/1538-4357/abd5b9","title":"Systematic Difference between Ionized and Molecular Gas Velocity Dispersions in z ∼ 1–2 Disks and Local Analogs","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Velocity dispersion; Star formation; Galaxy; Ionization; Redshift; Plasma","score_opus":0.009334485487175097,"score_gpt":0.23434362159863997,"score_spread":0.22500913611146486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119390322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99966276,0.00003442205,0.00006609899,0.0000033495917,6.1594875e-7,8.371448e-7,0.00009071744,0.000006276952,0.00013494151],"genre_scores_gemma":[0.99967337,0.000009465992,0.000048531347,0.0000020042135,0.0000014401458,7.833275e-7,0.0002281772,0.0000019753454,0.00003427141],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983287,0.000025163552,0.000011319453,0.000068819216,0.000032276515,0.000029524685],"domain_scores_gemma":[0.9993668,0.00014835891,0.00019997389,0.0000967648,0.00007711791,0.00011097409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038869478,0.00018180184,0.00021856067,0.0012431052,0.00021767555,0.00061620405,0.0003164677,0.00019863843,0.00067630643],"category_scores_gemma":[0.0010868163,0.00013929245,0.0001969541,0.0005364924,0.00025498576,0.00030158146,0.0004415963,0.00010348706,0.00018839592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009171243,0.000012084994,0.9932721,0.0000070368096,0.00005059164,0.000027557135,0.00013074977,0.0003457575,0.0037437729,0.0000648044,0.000048565333,0.0022052657],"study_design_scores_gemma":[0.0000029451207,0.00001417419,0.99852437,0.0000018182835,0.000013419303,0.000032281838,0.000088121466,0.0006678349,0.00054394256,0.000023020875,0.000086589454,0.0000015695242],"about_ca_topic_score_codex":0.0031108845,"about_ca_topic_score_gemma":0.00469134,"teacher_disagreement_score":0.0031108845,"about_ca_system_score_codex":0.00025200308,"about_ca_system_score_gemma":0.00006426559,"threshold_uncertainty_score":0.0061855316},"labels":[],"label_agreement":null},{"id":"W3119499817","doi":"10.3847/1538-4357/abd857","title":"Properties of Compact Faint Radio Sources as a Function of Angular Size from Stacking","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Polarization (electrochemistry); Cosmic microwave background; Angular diameter; Source counts; Galaxy; Radio galaxy; Population; Active galactic nucleus; Faraday effect","score_opus":0.009812330415883192,"score_gpt":0.19662335102714018,"score_spread":0.18681102061125698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119499817","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986332,0.00005130198,0.0004924981,0.000007212381,0.0000010588575,0.0000017745111,0.00033929746,0.000030088955,0.00044362425],"genre_scores_gemma":[0.99820876,0.00002868971,0.0002970637,0.0000032223024,0.000005279501,0.0000027660612,0.0013203053,0.000007840376,0.00012619441],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998535,0.000016160115,0.00001109159,0.00004488861,0.000037303966,0.000037059297],"domain_scores_gemma":[0.99782735,0.00066254224,0.00076256396,0.00026300078,0.00024132742,0.00024310933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041105758,0.00023987112,0.00026706338,0.001972836,0.00023087866,0.0008009063,0.00020791104,0.00017239492,0.001427366],"category_scores_gemma":[0.001690721,0.00017453784,0.00026164742,0.00089567446,0.00023554756,0.00030869397,0.00052790117,0.00016478034,0.0004109819],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025470386,0.000024905332,0.96196026,0.000017354998,0.00007365973,0.00010019175,0.00019814938,0.0019281815,0.024041299,0.00017490424,0.00015314716,0.011073323],"study_design_scores_gemma":[0.0000015430575,0.000019024357,0.99769455,0.0000015525711,0.000013698406,0.00010357564,0.000039257953,0.00087122835,0.0010694045,0.00006254896,0.000119941826,0.0000036948907],"about_ca_topic_score_codex":0.0009226583,"about_ca_topic_score_gemma":0.0009337265,"teacher_disagreement_score":0.001972836,"about_ca_system_score_codex":0.00015493153,"about_ca_system_score_gemma":0.00005111346,"threshold_uncertainty_score":0.0047749877},"labels":[],"label_agreement":null},{"id":"W3119565744","doi":"10.3847/1538-4357/acbb01","title":"Demographics of Protoplanetary Disks: A Simulated Population of Edge-on Systems","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Division of Astronomical Sciences; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of California, Los Angeles; Jet Propulsion Laboratory; Centre National de la Recherche Scientifique; Space Telescope Science Institute; European Southern Observatory; Queen's University; Eötvös Loránd Tudományegyetem; California Institute of Technology; European Commission; Los Alamos National Laboratory; Johns Hopkins University; Gordon and Betty Moore Foundation; Queen's University Belfast; National Aeronautics and Space Administration; Fundação de Amparo à Pesquisa do Estado de São Paulo; National Central University; Hungarian Scientific Research Fund; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Protoplanetary disk; Astrophysics; Planet; Population; Radiative transfer; Spectral energy distribution; Planetary system; Accretion (finance); Enhanced Data Rates for GSM Evolution; Astronomy; Galaxy; Computer science; Optics","score_opus":0.014463765210436796,"score_gpt":0.2523571589767729,"score_spread":0.23789339376633611,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119565744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987025,0.000025609957,0.0006229473,0.00004305499,0.0000026020414,0.0000148692925,0.00037346853,0.000014181858,0.00020077261],"genre_scores_gemma":[0.9976236,0.000028990442,0.00075343176,0.000028775647,0.000004030768,0.000023622191,0.0013025958,0.000007636474,0.00022732659],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996105,0.00012039136,0.000018852863,0.00014108492,0.000038066402,0.00007120521],"domain_scores_gemma":[0.9973072,0.0011720376,0.00033048878,0.00036694875,0.00033709322,0.00048628854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013063562,0.0003536194,0.00044583317,0.00069943676,0.00056307047,0.0009647448,0.0015314603,0.001056942,0.001384947],"category_scores_gemma":[0.004225207,0.00028376593,0.0005020842,0.0005490727,0.00065258634,0.0007628553,0.0008282859,0.00074736,0.00037698075],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051799807,0.00047718696,0.66711724,0.00004114244,0.00017441344,0.00050113915,0.0006290689,0.3180408,0.002256356,0.0031169306,0.0018368339,0.0052909115],"study_design_scores_gemma":[0.00013821249,0.00038710306,0.10388059,0.00003000459,0.00007407131,0.00036382175,0.0008018564,0.88898987,0.0009888111,0.0032908106,0.0010063783,0.000048497626],"about_ca_topic_score_codex":0.008042849,"about_ca_topic_score_gemma":0.0073173107,"teacher_disagreement_score":0.008042849,"about_ca_system_score_codex":0.0008094581,"about_ca_system_score_gemma":0.00043510328,"threshold_uncertainty_score":0.015992045},"labels":[],"label_agreement":null},{"id":"W3119602371","doi":"10.3847/1538-4357/abd6e4","title":"ALMA 1.3 mm Survey of Lensed Submillimeter Galaxies Selected by Herschel: Discovery of Spatially Extended SMGs and Implications","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Thailand Science Research and Innovation","keywords":"Galaxy; Surface brightness; Star formation; Brightness; Galaxy formation and evolution; Luminous infrared galaxy","score_opus":0.010023052253177537,"score_gpt":0.2210479897063699,"score_spread":0.21102493745319237,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119602371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99891686,0.00013026428,0.00013208417,0.000030336856,0.0000013406839,0.0000023271646,0.00040030698,0.000029065004,0.0003574223],"genre_scores_gemma":[0.99911445,0.000040424457,0.00025516926,0.000019280566,0.000007959531,0.0000023520568,0.0004503116,0.0000041391327,0.00010588557],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997042,0.000052701598,0.000011914306,0.000092418886,0.00007279004,0.00006598748],"domain_scores_gemma":[0.9988588,0.00014037002,0.0005089403,0.00010890571,0.00011587139,0.00026719194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005353285,0.00023073782,0.0003013501,0.0017294843,0.00030095386,0.0005152937,0.00038046227,0.0002176876,0.00116424],"category_scores_gemma":[0.000652287,0.00013529974,0.0003044571,0.0009066111,0.0002183607,0.0003056183,0.0005330403,0.00021239123,0.00027357557],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048446633,0.000017495197,0.9911876,0.000010391947,0.000040557505,0.000070743255,0.00009020923,0.000118172735,0.0042750053,0.00007375635,0.00019811094,0.003869556],"study_design_scores_gemma":[0.0000018537592,0.000011103881,0.9993352,0.0000018257365,0.0000051263164,0.0000472283,0.000034097295,0.00019886986,0.0001728431,0.000019421588,0.00017093681,0.0000015226664],"about_ca_topic_score_codex":0.0070470823,"about_ca_topic_score_gemma":0.012038843,"teacher_disagreement_score":0.0070470823,"about_ca_system_score_codex":0.00044695506,"about_ca_system_score_gemma":0.0001362873,"threshold_uncertainty_score":0.014012158},"labels":[],"label_agreement":null},{"id":"W3119705783","doi":"10.3847/1538-4357/abdb27","title":"The Evolution of the IR Luminosity Function and Dust-obscured Star Formation over the Past 13 Billion Years","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":174,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Institutes of Natural Sciences; Comisión Nacional de Investigación Científica y Tecnológica; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Astronomical Observatory of Japan; Danmarks Grundforskningsfond; Max-Planck-Gesellschaft; Knut och Alice Wallenbergs Stiftelse; University of Toronto; National Research Foundation; National Radio Astronomy Observatory; Villum Fonden; Research Corporation for Science Advancement; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Star formation; Reionization; Billion years; Luminosity function; Galaxy; Galaxy formation and evolution; Luminosity; Redshift; Stellar mass; Milky Way","score_opus":0.005672442320949819,"score_gpt":0.1871354087406848,"score_spread":0.18146296641973497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119705783","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979328,0.00035025735,0.00012956903,0.00012462302,0.0000042143865,0.0000013335932,0.0008843381,0.000013998299,0.00055885065],"genre_scores_gemma":[0.9987419,0.00013836553,0.000097335134,0.00002329387,0.00001126246,0.0000018710411,0.0006994605,0.000003370972,0.00028310867],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998419,0.000026891134,0.000011976534,0.00004779324,0.000036038196,0.000035456982],"domain_scores_gemma":[0.9983374,0.00019875467,0.00093729846,0.00009532507,0.00020421974,0.0002269789],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042735515,0.00015958976,0.00016756548,0.0010739772,0.00019521681,0.0006258523,0.00026954673,0.0003811729,0.0014575975],"category_scores_gemma":[0.0017760103,0.0001225856,0.00030575093,0.00079729117,0.00022697085,0.00045316067,0.0003988268,0.00031959426,0.0003633503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000025917123,0.000013226673,0.9959013,0.000006838454,0.000039165945,0.00006021925,0.00007692146,0.0002527614,0.00053795765,0.000083404666,0.000180174,0.0028221207],"study_design_scores_gemma":[4.408559e-7,0.000007978414,0.9992131,0.0000023588284,0.00000720312,0.00006689698,0.000029239485,0.00027919447,0.00007797909,0.000025394984,0.00028874935,0.0000014972492],"about_ca_topic_score_codex":0.0058937278,"about_ca_topic_score_gemma":0.0058917366,"teacher_disagreement_score":0.0058937278,"about_ca_system_score_codex":0.00042081325,"about_ca_system_score_gemma":0.00011544985,"threshold_uncertainty_score":0.011718869},"labels":[],"label_agreement":null},{"id":"W3119868608","doi":"10.3847/1538-4357/ac043c","title":"Star Formation in a Strongly Magnetized Cloud","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"European Research Council; National Science Foundation","keywords":"Protein filament; Physics; Astrophysics; Protostar; Submillimeter Array; Molecular cloud; Millimeter; Star formation; Magnetic field; Polarization (electrochemistry); Stars","score_opus":0.010368996763573222,"score_gpt":0.23421184201905215,"score_spread":0.22384284525547893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119868608","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997837,0.000016077563,0.000022201091,0.000016181408,6.823414e-7,0.0000021729313,0.000029834458,0.0000013163153,0.00012781793],"genre_scores_gemma":[0.9998153,0.000013153763,0.000027402457,0.0000075779503,0.0000026336895,0.0000011965432,0.00006935967,7.1022083e-7,0.00006271797],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99991465,0.000013587433,0.000002711173,0.000018802893,0.000010867573,0.0000393652],"domain_scores_gemma":[0.9997625,0.000033853903,0.00007442999,0.000009958508,0.000012792026,0.00010651278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012062985,0.00019958483,0.00023500719,0.0002921503,0.00059370167,0.0005472622,0.00027610868,0.0002701042,0.00071446603],"category_scores_gemma":[0.00035688165,0.00009809996,0.00013144451,0.00029239745,0.0003261558,0.0001807566,0.0004076265,0.0002073589,0.00011141698],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000498544,0.00034156482,0.9651289,0.000021368873,0.00006783875,0.0019434755,0.0004240797,0.008224616,0.01854988,0.000983636,0.0006912003,0.003124808],"study_design_scores_gemma":[0.000104209066,0.0002572299,0.9665775,0.000008598288,0.000025082096,0.0004315319,0.0007148625,0.02935729,0.0011674335,0.0005106512,0.0008324228,0.0000132384785],"about_ca_topic_score_codex":0.01942462,"about_ca_topic_score_gemma":0.014657792,"teacher_disagreement_score":0.01942462,"about_ca_system_score_codex":0.0006894443,"about_ca_system_score_gemma":0.00028578565,"threshold_uncertainty_score":0.038623095},"labels":[],"label_agreement":null},{"id":"W3119895874","doi":"10.3847/1538-4357/abdbb4","title":"The Polar Precursor Method for Solar Cycle Prediction: Comparison of Predictors and Their Temporal Range","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Collège de Bois-de-Boulogne","funders":"","keywords":"Polar; Amplitude; Solar dynamo; Solar cycle; Dynamo; Solar observatory; Flux (metallurgy); Solar minimum; Solar cycle 24; Sunspot","score_opus":0.010122019875312391,"score_gpt":0.2661006954578195,"score_spread":0.2559786755825071,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3119895874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8327209,0.0020540152,0.1546728,0.0005064146,0.00014621968,0.00013973005,0.0029533552,0.0023534358,0.004453065],"genre_scores_gemma":[0.96516913,0.00034756307,0.030423265,0.000053461186,0.00007688938,0.000073994444,0.003006654,0.0001556144,0.0006934539],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986767,0.0007743416,0.0000733314,0.00022831673,0.00016711181,0.00008006276],"domain_scores_gemma":[0.98225635,0.014455246,0.000718465,0.00085119053,0.0013556718,0.00036294624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007815242,0.00084061053,0.0007237025,0.0019903053,0.00040507864,0.0011562047,0.00063526724,0.0005274495,0.0020587202],"category_scores_gemma":[0.015879782,0.00028041436,0.00054673565,0.0014548628,0.00033419128,0.0009841936,0.0008130969,0.0011540393,0.00063410366],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021329,0.00029701262,0.44028428,0.00016806037,0.00062556565,0.0001860353,0.00019176376,0.34289283,0.0016427,0.0019076539,0.004210545,0.2054606],"study_design_scores_gemma":[0.000026988482,0.00014744495,0.017088965,0.00003486748,0.00004949741,0.000040430754,0.00008575531,0.98072493,0.0007227402,0.0005256578,0.0005339515,0.000018820954],"about_ca_topic_score_codex":0.011391076,"about_ca_topic_score_gemma":0.0067265346,"teacher_disagreement_score":0.011391076,"about_ca_system_score_codex":0.0002705181,"about_ca_system_score_gemma":0.00124882,"threshold_uncertainty_score":0.04133147},"labels":[],"label_agreement":null},{"id":"W3120734955","doi":"10.3847/1538-4357/ac2bff","title":"Wolf-Rayet Galaxies in SDSS-IV MaNGA. II. Metallicity Dependence of the High-mass Slope of the Stellar Initial Mass Function","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Key Research and Development Program of China; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Metallicity; Astrophysics; Initial mass function; Galaxy; Stellar population; Stellar mass; Population; Star formation","score_opus":0.00874306218994117,"score_gpt":0.20783096702116743,"score_spread":0.19908790483122626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3120734955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990627,0.000054542434,0.00007291377,0.000008100625,8.373384e-7,0.000002252008,0.0004447353,0.00001735463,0.0003365947],"genre_scores_gemma":[0.998694,0.000016414353,0.000099839286,0.0000048045085,0.0000018050598,0.000002744741,0.0010488208,0.000007263999,0.00012437708],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997626,0.000041973213,0.00001648989,0.00009228099,0.000034124765,0.000052647065],"domain_scores_gemma":[0.9984478,0.00037044857,0.00056893437,0.00021287239,0.0001282734,0.0002716496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056130614,0.00029449575,0.0001849381,0.0016967787,0.00025905893,0.0005642726,0.00025307553,0.0002800112,0.001304678],"category_scores_gemma":[0.0012138088,0.00017866763,0.00029781702,0.0007400334,0.00032118292,0.00032413536,0.0004629236,0.00016171164,0.0006929748],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006876364,0.000018652125,0.9944325,0.000008989993,0.00002569218,0.00004224048,0.00008074152,0.0005377281,0.0030488798,0.00009464041,0.000095108284,0.0015461047],"study_design_scores_gemma":[0.0000019971687,0.000009543311,0.99878424,0.0000020355264,0.000004184551,0.00002502159,0.000031074906,0.0007513113,0.00027971415,0.00002909678,0.000080405014,0.0000014364381],"about_ca_topic_score_codex":0.0026657777,"about_ca_topic_score_gemma":0.0036369646,"teacher_disagreement_score":0.0026657777,"about_ca_system_score_codex":0.00029584934,"about_ca_system_score_gemma":0.00008046885,"threshold_uncertainty_score":0.0053004622},"labels":[],"label_agreement":null},{"id":"W3120805134","doi":"10.3847/1538-4357/abddbe","title":"The Star Formation History of Eridanus II: On the Role of Supernova Feedback in the Quenching of Ultrafaint Dwarf Galaxies*","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Horizon 2020 Framework Programme; Max-Planck-Gesellschaft; Space Telescope Science Institute; Agencia Estatal de Investigación; Norges Forskningsråd; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Star formation; Globular cluster; Astronomy; Galaxy; Virial mass; Milky Way; Dwarf galaxy; Stellar mass; Population; Galaxy cluster","score_opus":0.008273427304251613,"score_gpt":0.19263574713719653,"score_spread":0.1843623198329449,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3120805134","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99908936,0.00016077548,0.00021215343,0.00000797722,0.0000010738091,0.0000016552694,0.00004876942,0.00000764442,0.0004705972],"genre_scores_gemma":[0.99972266,0.000030576703,0.000069547634,0.000003686969,0.000001349119,9.042642e-7,0.000045059216,0.0000016176092,0.00012451372],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999405,0.000007055209,0.0000055811133,0.000024801673,0.0000096546555,0.000012340075],"domain_scores_gemma":[0.9996966,0.000049437425,0.00011992331,0.000030112207,0.00003478646,0.000069162066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022545847,0.00019014173,0.00018628508,0.000324589,0.00015631453,0.00031880487,0.0002631184,0.0001434987,0.00066448055],"category_scores_gemma":[0.00040541028,0.000081590406,0.00013242252,0.00013273807,0.00017781174,0.00018499365,0.00027948472,0.0000985207,0.00012414117],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020044416,0.00005404047,0.8501632,0.000057627476,0.000047874193,0.0001681444,0.00019796596,0.0013903383,0.13347392,0.00055367954,0.00007969757,0.013613062],"study_design_scores_gemma":[0.000003904933,0.00009489847,0.98846275,0.0000050799044,0.0000163908,0.00010545124,0.00006340197,0.003689626,0.006991891,0.00020962323,0.00035288726,0.0000040455056],"about_ca_topic_score_codex":0.0019159976,"about_ca_topic_score_gemma":0.001704884,"teacher_disagreement_score":0.0019159976,"about_ca_system_score_codex":0.0002842525,"about_ca_system_score_gemma":0.000086659325,"threshold_uncertainty_score":0.0038096905},"labels":[],"label_agreement":null},{"id":"W3121052157","doi":"10.3847/1538-4357/abfcd3","title":"The NANOGrav 11 yr Data Set: Limits on Supermassive Black Hole Binaries in Galaxies within 500 Mpc","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"","keywords":"Gravitational wave; Supermassive black hole; Galaxy; Redshift; Milky Way; Observatory; Binary black hole; Mass ratio; Pulsar; Black hole (networking)","score_opus":0.02023047212716363,"score_gpt":0.24168833892328515,"score_spread":0.2214578667961215,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3121052157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9460682,0.00036751147,0.002014687,0.00011084647,0.000017874143,0.00004224953,0.04465816,0.00020087943,0.006519685],"genre_scores_gemma":[0.90417945,0.000110912806,0.002149038,0.00007972029,0.000019877607,0.000045244913,0.09246517,0.000032250853,0.00091830804],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993255,0.00009116697,0.00007858972,0.00021559236,0.00020672525,0.00008239101],"domain_scores_gemma":[0.99760336,0.00074644486,0.0004845934,0.0006041134,0.00031465592,0.0002468018],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009797384,0.0002937798,0.00037904945,0.0026188316,0.0002893059,0.0007827228,0.000540518,0.0003328241,0.0017493006],"category_scores_gemma":[0.0027312292,0.00017707272,0.00034354406,0.0016032081,0.000202791,0.0005139345,0.0012199502,0.00018439806,0.0006394485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002895056,0.00006152706,0.9684997,0.0001094786,0.000115877745,0.00013135115,0.00014738813,0.0043852585,0.0049773045,0.0008531416,0.0045157126,0.015913649],"study_design_scores_gemma":[0.000026382026,0.0000474804,0.97795266,0.000025646483,0.00004392702,0.00010926716,0.0000992073,0.006804134,0.0028950362,0.00026513875,0.011716665,0.0000144574105],"about_ca_topic_score_codex":0.011070531,"about_ca_topic_score_gemma":0.01894382,"teacher_disagreement_score":0.011070531,"about_ca_system_score_codex":0.00032610513,"about_ca_system_score_gemma":0.00023299898,"threshold_uncertainty_score":0.022012174},"labels":[],"label_agreement":null},{"id":"W3121689307","doi":"10.1088/0004-637x/813/1/65","title":"THE NANOGRAV NINE-YEAR DATA SET: OBSERVATIONS, ARRIVAL TIME MEASUREMENTS, AND ANALYSIS OF 37 MILLISECOND PULSARS","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":218,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Vancouver Coastal Health; McGill University; University of British Columbia","funders":"","keywords":"Pulsar; Millisecond pulsar; Static timing analysis; Observatory; Time of arrival; Noise (video); Gravitational wave; Pulse (music); Millisecond","score_opus":0.09360699327757842,"score_gpt":0.347644920936201,"score_spread":0.25403792765862254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3121689307","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9417573,0.00037312348,0.00627531,0.00023296625,0.00007097904,0.0000974038,0.044542346,0.00038308342,0.0062675322],"genre_scores_gemma":[0.85586435,0.00040399967,0.019405022,0.00021811487,0.00010515028,0.00018222339,0.1210965,0.00020948556,0.0025151852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996629,0.000030115414,0.00003539449,0.000089765876,0.00014992525,0.00003191003],"domain_scores_gemma":[0.9985453,0.00017865073,0.00038524042,0.00039214297,0.00033656252,0.00016226716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006935717,0.0002777708,0.0003151315,0.0017973686,0.00050245645,0.00045354763,0.00057542423,0.00035258007,0.00093837525],"category_scores_gemma":[0.0012082793,0.00020338566,0.00028537915,0.0018915883,0.00022897078,0.00043778346,0.00087141595,0.00049761054,0.00060012756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011270329,0.0004996206,0.81761533,0.00035341815,0.00041130328,0.0007847706,0.000875012,0.008972996,0.065621056,0.0020657848,0.019817967,0.08185581],"study_design_scores_gemma":[0.00008314422,0.00014601396,0.95471454,0.000024429604,0.00008823822,0.00043965384,0.00012653014,0.0050717895,0.0063824807,0.00046426427,0.03240998,0.00004878906],"about_ca_topic_score_codex":0.007497583,"about_ca_topic_score_gemma":0.024504049,"teacher_disagreement_score":0.007497583,"about_ca_system_score_codex":0.00035501752,"about_ca_system_score_gemma":0.00046930363,"threshold_uncertainty_score":0.0149078965},"labels":[],"label_agreement":null},{"id":"W3121694496","doi":"10.3847/1538-4357/abf9a3","title":"Dark Matter Constraints from a Unified Analysis of Strong Gravitational Lenses and Milky Way Satellite Galaxies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Dark matter; Gravitational lens; Satellite galaxy; Halo; Weak gravitational lensing; Galaxy; Milky Way; Population; Strong gravitational lensing","score_opus":0.010299638463379427,"score_gpt":0.2295045039967431,"score_spread":0.21920486553336369,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3121694496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927793,0.000101579506,0.006368783,0.00003857822,0.0000012636506,0.0000036774627,0.0001030014,0.000026273234,0.0005775643],"genre_scores_gemma":[0.9987722,0.000023123284,0.0010519383,0.000006220503,0.0000033185636,0.0000021383673,0.000087873574,0.000004063481,0.000049094448],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994469,0.00019067164,0.0000425409,0.00011250657,0.00013182736,0.0000756269],"domain_scores_gemma":[0.99648076,0.0013988769,0.0011129618,0.0005234971,0.00020296047,0.00028094125],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014792356,0.00057659886,0.00048001413,0.001492644,0.000299945,0.0016587916,0.00045920085,0.0002608332,0.0006429131],"category_scores_gemma":[0.004211794,0.00040620042,0.0009903617,0.0009199586,0.00072622206,0.000744649,0.0021331059,0.00036505715,0.000081303035],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003059077,0.000032860178,0.9319194,0.00004896839,0.0008487524,0.0002975065,0.00017981244,0.018815223,0.022967046,0.008596197,0.00013909809,0.015849214],"study_design_scores_gemma":[0.000035973353,0.00012325933,0.83515596,0.000021572809,0.00028784075,0.00016444104,0.00035459595,0.13988106,0.009464427,0.0138096595,0.0006577723,0.000043353022],"about_ca_topic_score_codex":0.0041708723,"about_ca_topic_score_gemma":0.0054252734,"teacher_disagreement_score":0.0041708723,"about_ca_system_score_codex":0.0004636947,"about_ca_system_score_gemma":0.0005338946,"threshold_uncertainty_score":0.008293152},"labels":[],"label_agreement":null},{"id":"W3121941021","doi":"10.3847/1538-4357/abddb1","title":"FAUST. II. Discovery of a Secondary Outflow in IRAS 15398−3359: Variability in Outflow Direction during the Earliest Stage of Star Formation?","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Outflow; Star formation; Accretion (finance); Bipolar outflow; Molecular cloud; Herbig–Haro object; Line (geometry)","score_opus":0.00716535327658494,"score_gpt":0.22604501581558242,"score_spread":0.2188796625389975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3121941021","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98549193,0.00006731284,0.0006133044,0.00008277252,0.000009051659,0.000026202686,0.010456206,0.0008566328,0.002396606],"genre_scores_gemma":[0.97924167,0.000025787853,0.0033809068,0.000037115533,0.0000058518895,0.000022828739,0.016155407,0.00011573782,0.0010146241],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989295,0.000011401174,0.0000045222373,0.000031639527,0.000028008806,0.000031481362],"domain_scores_gemma":[0.9995115,0.00005598041,0.00015936632,0.00007791911,0.000082565086,0.00011263773],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028717588,0.00020879848,0.0001384356,0.0007695338,0.0003951975,0.00031935336,0.0002683252,0.00016077116,0.0012959137],"category_scores_gemma":[0.000551401,0.00012143566,0.00015527659,0.0005826695,0.00016630102,0.00014070857,0.00019972894,0.00018540917,0.00073296245],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010804423,0.00021240911,0.857808,0.00008801137,0.00010010615,0.0010165616,0.00084789784,0.0019687065,0.07275546,0.00042510655,0.013474379,0.050222892],"study_design_scores_gemma":[0.000016565435,0.00004854956,0.9881252,0.000006125454,0.000010082902,0.00021813565,0.00006887483,0.0022692028,0.003639032,0.000039171904,0.00555141,0.000007723224],"about_ca_topic_score_codex":0.028097678,"about_ca_topic_score_gemma":0.049652353,"teacher_disagreement_score":0.028097678,"about_ca_system_score_codex":0.0004792193,"about_ca_system_score_gemma":0.00018240469,"threshold_uncertainty_score":0.055868268},"labels":[],"label_agreement":null},{"id":"W3122690528","doi":"10.3847/1538-4357/abdf5c","title":"The Fast-evolving Type Ib Supernova SN 2015dj in NGC 7371","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Ejecta; Light curve; Supernova; Physics; Astrophysics; Kinetic energy; Binary number; Type (biology); Mathematics","score_opus":0.012144490105136008,"score_gpt":0.2400683664642978,"score_spread":0.22792387635916178,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3122690528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981188,0.00018442827,0.0001392374,0.0000146412085,0.000006255059,0.000004122864,0.0006863051,0.000020353278,0.000825708],"genre_scores_gemma":[0.99897456,0.000041603234,0.00011431865,0.0000066733037,0.0000038159747,0.0000020461662,0.0006524719,0.0000030701367,0.0002014784],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999057,0.0000045879333,0.000004817614,0.000017398734,0.00002437443,0.00004325408],"domain_scores_gemma":[0.9997253,0.00002258953,0.00007166045,0.000020368529,0.000057998535,0.00010208069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013504697,0.00030912337,0.00028741034,0.0011371229,0.0005727726,0.00069961214,0.00020544874,0.00020715002,0.00063953147],"category_scores_gemma":[0.00026804855,0.00010932203,0.00027573985,0.0008384027,0.0002580406,0.00013557558,0.0003360121,0.00020801813,0.0002249869],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033904068,0.00007566428,0.95062256,0.000037614212,0.00012740413,0.0036011583,0.00023868989,0.0016327648,0.025664188,0.00032766754,0.0010182444,0.016315173],"study_design_scores_gemma":[0.000001940892,0.000034430344,0.99723536,0.0000039257416,0.000020126681,0.0006311836,0.0001310382,0.00034382765,0.0006688244,0.00004512363,0.00087778084,0.0000064909245],"about_ca_topic_score_codex":0.0688767,"about_ca_topic_score_gemma":0.09510725,"teacher_disagreement_score":0.0688767,"about_ca_system_score_codex":0.0011850913,"about_ca_system_score_gemma":0.0004117156,"threshold_uncertainty_score":0.13695157},"labels":[],"label_agreement":null},{"id":"W3122816601","doi":"10.3847/1538-4357/ac356c","title":"Hubble Space Telescope Imaging of Isolated Local Volume Dwarfs GALFA Dw3 and Dw4","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Division of Grants and Agreements; Division of Astronomical Sciences; National Aeronautics and Space Administration; Universities Space Research Association; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Galaxy; Algorithm; Red-giant branch; Astrophysics; Computer science; Metallicity","score_opus":0.004083795632725807,"score_gpt":0.1927409806851932,"score_spread":0.18865718505246737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3122816601","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942116,0.000057147445,0.0005006476,0.000051983796,0.0000055377823,0.0000075223243,0.0015176896,0.00014661145,0.0035012118],"genre_scores_gemma":[0.9950631,0.000032659835,0.0013334571,0.00005164505,0.000008530202,0.0000094393,0.002255035,0.000031698833,0.0012143159],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999229,0.000004566082,0.000002355361,0.00001807518,0.00001971234,0.00003246518],"domain_scores_gemma":[0.9997509,0.000027340839,0.000041690124,0.000034770936,0.00004270267,0.00010260831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014711243,0.00016743547,0.00015599723,0.0011830003,0.00027411996,0.00036236426,0.0002836188,0.00026653937,0.001767162],"category_scores_gemma":[0.00020939518,0.00013436453,0.0002716297,0.00052412105,0.00016578313,0.00015760298,0.00031602147,0.00022489102,0.00044855115],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011473587,0.00022351467,0.58111227,0.000089525274,0.00018801443,0.00078500056,0.00090422237,0.0020305114,0.34378543,0.0008461287,0.008541511,0.060346577],"study_design_scores_gemma":[0.000024532632,0.000057229427,0.98794055,0.000006295606,0.000019483889,0.00022152494,0.00017893827,0.0016476087,0.0064114,0.00014430405,0.0033375218,0.000010658771],"about_ca_topic_score_codex":0.010469792,"about_ca_topic_score_gemma":0.022091867,"teacher_disagreement_score":0.010469792,"about_ca_system_score_codex":0.0005113503,"about_ca_system_score_gemma":0.00014290363,"threshold_uncertainty_score":0.020817697},"labels":[],"label_agreement":null},{"id":"W3123194088","doi":"10.3847/1538-4357/abddc1","title":"A Spatially Resolved Survey of Distant Quasar Host Galaxies. II. Photoionization and Kinematics of the ISM","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Quasar; Supermassive black hole; Galaxy; Velocity dispersion; Photoionization; Active galactic nucleus; Redshift; Star formation; Radio galaxy","score_opus":0.009892174767860243,"score_gpt":0.21119200357684362,"score_spread":0.20129982880898337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3123194088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99886537,0.00018322511,0.00011467466,0.000018101511,0.0000012039412,0.0000040126706,0.00035794708,0.000008903959,0.0004466462],"genre_scores_gemma":[0.99876803,0.00010659371,0.00024170193,0.000016899046,0.0000071837526,0.00000315715,0.0005812118,0.0000027097667,0.0002725496],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987876,0.000014768955,0.000007886277,0.000040353385,0.000027932067,0.000030379075],"domain_scores_gemma":[0.9996075,0.000034144177,0.00015450772,0.000032860346,0.00004772934,0.0001231264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017140999,0.0001777314,0.00018070337,0.0011583252,0.00026577758,0.0003437069,0.00016166584,0.00017787365,0.0012001158],"category_scores_gemma":[0.00027130617,0.00015410424,0.00013969188,0.00068443356,0.00013780882,0.00031262237,0.0004191993,0.0001813688,0.00046896868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004552885,0.000048426908,0.9695304,0.000023100903,0.00004277072,0.00013162881,0.00037692493,0.00009492049,0.021109374,0.000104674764,0.00018586392,0.008306462],"study_design_scores_gemma":[0.0000015963637,0.00002568687,0.9991135,0.00000195273,0.000005830942,0.00012324713,0.00007157801,0.00005162306,0.00027675653,0.0000106070365,0.00031644167,0.0000011182913],"about_ca_topic_score_codex":0.003850532,"about_ca_topic_score_gemma":0.008843915,"teacher_disagreement_score":0.003850532,"about_ca_system_score_codex":0.0001379024,"about_ca_system_score_gemma":0.00008661471,"threshold_uncertainty_score":0.0076562166},"labels":[],"label_agreement":null},{"id":"W3123197276","doi":"10.3847/1538-4357/abe942","title":"Benchmarking Dust Emission Models in M101","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Science Foundation","keywords":"Black-body radiation; Milky Way; Metallicity; Photometry (optics); Cosmic dust; Range (aeronautics); Cirrus","score_opus":0.01094728982065001,"score_gpt":0.21879287672024927,"score_spread":0.20784558689959926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3123197276","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99212307,0.00009362072,0.0054559396,0.00007832904,0.000007355565,0.00001970707,0.00033155427,0.00021868655,0.0016718006],"genre_scores_gemma":[0.996476,0.000035552537,0.002530927,0.000019935236,0.0000037284171,0.000018871442,0.00059094076,0.000051979856,0.00027204762],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99971694,0.000089477224,0.0000171032,0.000096040836,0.000041244923,0.000039164555],"domain_scores_gemma":[0.9991769,0.00047892425,0.00006736491,0.00011083361,0.0000898225,0.00007611477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007900843,0.0006881649,0.0005627984,0.0006995988,0.00035814955,0.0011593308,0.0014123343,0.0009766639,0.000951343],"category_scores_gemma":[0.0017862236,0.00032855922,0.00095602695,0.00059461367,0.0003937484,0.0005462296,0.00040282472,0.00025994817,0.0003294789],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017028942,0.0001436287,0.04436591,0.000046507852,0.0001143617,0.00013255654,0.0001169494,0.9463458,0.0022776662,0.0013042735,0.00032245065,0.004659476],"study_design_scores_gemma":[0.00006832797,0.000098040735,0.01670483,0.000009400164,0.000029911032,0.00004725782,0.000085488515,0.9801543,0.0013115193,0.00096461765,0.00050958444,0.000016798725],"about_ca_topic_score_codex":0.016123837,"about_ca_topic_score_gemma":0.008847054,"teacher_disagreement_score":0.016123837,"about_ca_system_score_codex":0.0019596256,"about_ca_system_score_gemma":0.00050396664,"threshold_uncertainty_score":0.032059968},"labels":[],"label_agreement":null},{"id":"W3123399237","doi":"10.3847/1538-4357/abdeb7","title":"Massive White Dwarfs in Young Star Clusters","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; European Space Agency","keywords":"White dwarf; Astrometry; Open cluster; Physics; Astrophysics; Cluster (spacecraft); Sky; Star cluster; Sigma; Galaxy cluster; Stars; Astronomy; Galaxy; Computer science","score_opus":0.008622315177319049,"score_gpt":0.21905610567278658,"score_spread":0.21043379049546754,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3123399237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980063,0.00015061813,0.0007883483,0.000013933254,0.000004041847,0.000011069124,0.00029110836,0.000032299322,0.00070231623],"genre_scores_gemma":[0.9974376,0.00006489526,0.001129492,0.0000111876725,0.000005547534,0.000006776935,0.00094886037,0.0000068111717,0.00038878794],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994815,0.00008118738,0.000043483837,0.00014893137,0.00014527286,0.00009966581],"domain_scores_gemma":[0.9987527,0.000297434,0.00033461055,0.0001495428,0.0001825057,0.0002831873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010318087,0.00027648723,0.00039039168,0.002177041,0.0006121831,0.00086328655,0.0004728801,0.00019513644,0.00074672676],"category_scores_gemma":[0.0022263804,0.00013847243,0.00019030062,0.0015292998,0.00027347804,0.00040892433,0.0009898216,0.00017371566,0.0003609197],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002425863,0.000064128966,0.97213453,0.000045519933,0.00004931999,0.00039000818,0.0005429586,0.00194585,0.012681223,0.00071857317,0.00044576157,0.010739499],"study_design_scores_gemma":[0.000013171911,0.00015886592,0.9864071,0.000014234655,0.000039572136,0.0003648173,0.00048074964,0.0034503024,0.004556695,0.00067608384,0.0038207285,0.000017714436],"about_ca_topic_score_codex":0.0060357214,"about_ca_topic_score_gemma":0.006813418,"teacher_disagreement_score":0.0060357214,"about_ca_system_score_codex":0.00031849198,"about_ca_system_score_gemma":0.00045572975,"threshold_uncertainty_score":0.012001157},"labels":[],"label_agreement":null},{"id":"W3124139452","doi":"10.3847/1538-4357/abe0b4","title":"Tracing Young Star-forming Clumps in the Nearby Flocculent Spiral Galaxy NGC 7793 with UVIT Imaging","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Galaxy; Spiral galaxy; Star formation; Star cluster; Cluster (spacecraft); Stellar mass; Telescope; Mass distribution; Irregular galaxy; Milky Way","score_opus":0.006817616447650402,"score_gpt":0.2098191810486486,"score_spread":0.2030015646009982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3124139452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985343,0.000105750034,0.00045533455,0.00000980219,0.0000014011514,0.0000040958253,0.00016819654,0.00003777249,0.0006833237],"genre_scores_gemma":[0.9985392,0.00004500184,0.0010651042,0.000008478197,0.000003851622,0.000003006253,0.00020381152,0.0000060343723,0.00012553806],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999362,0.000005108004,0.0000031782656,0.000014481837,0.000019139741,0.000021722157],"domain_scores_gemma":[0.99975353,0.000025881089,0.00007687146,0.000026306541,0.000039400435,0.00007790053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014524316,0.00017565076,0.00016814198,0.0016768066,0.00023890202,0.00041923227,0.00034039075,0.00021715835,0.00048532835],"category_scores_gemma":[0.00024840483,0.00013689543,0.00019313801,0.000682472,0.0001624612,0.0001727016,0.00039423344,0.00013308457,0.00016557635],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017830123,0.00006861662,0.8103525,0.0000760129,0.000096482225,0.0014688469,0.00088160776,0.0020337924,0.16120951,0.0003522411,0.0005808768,0.022701252],"study_design_scores_gemma":[0.000004191584,0.000045047665,0.9879353,0.000017743218,0.00003618453,0.0004806865,0.00034309193,0.005413735,0.0048755966,0.000074763884,0.00076622015,0.000007448473],"about_ca_topic_score_codex":0.004290711,"about_ca_topic_score_gemma":0.0074248924,"teacher_disagreement_score":0.004290711,"about_ca_system_score_codex":0.00028477877,"about_ca_system_score_gemma":0.00008773812,"threshold_uncertainty_score":0.008531451},"labels":[],"label_agreement":null},{"id":"W3124918126","doi":"10.3847/1538-4357/abdfc5","title":"ALMA Observation of the Protoplanetary Disk around WW Cha: Faint Double-peaked Ring and Asymmetric Structure","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Radiative transfer; Spectral index; Wavelength; Spectral energy distribution; Protoplanetary disk; Monte Carlo method; Spiral galaxy; Stars; Debris disk","score_opus":0.014628805775544275,"score_gpt":0.22574957578555246,"score_spread":0.2111207700100082,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3124918126","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99755967,0.000056405126,0.000525134,0.000033749493,0.000008116457,0.000007756382,0.00038305277,0.000061809,0.0013643724],"genre_scores_gemma":[0.9985474,0.00001886517,0.00076290313,0.000012633639,0.000012323187,0.000004830185,0.0003940542,0.000004179228,0.00024279383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999948,0.0000060703915,0.0000023222467,0.000014277146,0.000016392247,0.000012860201],"domain_scores_gemma":[0.99985445,0.000015614434,0.000028690978,0.000015416927,0.00002515999,0.000060677892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000104320214,0.00015452685,0.0001741022,0.00060533156,0.00036465505,0.00028579982,0.0002907917,0.00030502887,0.0010780704],"category_scores_gemma":[0.00018933702,0.00010381253,0.00020982807,0.00023345015,0.00013176678,0.00015855426,0.0002857268,0.00026781508,0.00022497747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062791974,0.00023367892,0.72838,0.00010225182,0.00019330363,0.0020769737,0.0005001283,0.0036969308,0.24471454,0.00044303085,0.0014178576,0.017613273],"study_design_scores_gemma":[0.000030251402,0.00011645623,0.9853491,0.000007863018,0.000035346064,0.00036873174,0.00010756695,0.0078121442,0.004541629,0.00010176157,0.001519071,0.000010059764],"about_ca_topic_score_codex":0.003738264,"about_ca_topic_score_gemma":0.00716404,"teacher_disagreement_score":0.003738264,"about_ca_system_score_codex":0.00020738856,"about_ca_system_score_gemma":0.000082737926,"threshold_uncertainty_score":0.007432997},"labels":[],"label_agreement":null},{"id":"W3125615034","doi":"10.3847/1538-4357/abd474","title":"The Extraordinary Outburst in the Massive Protostellar System NGC 6334 I-MM1: Spatiokinematics of Water Masers during a Contemporaneous Flare Event","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Maser; Physics; Astrophysics; Proper motion; Outflow; Very-long-baseline interferometry; Accretion (finance); Astronomy; Jet (fluid); Very Long Baseline Array; Position angle; Shock (circulatory); Bow shock (aerodynamics); Stars; Shock wave; Quasar; Galaxy","score_opus":0.00791763377740574,"score_gpt":0.22302130474974857,"score_spread":0.21510367097234284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3125615034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99974924,0.0000146116845,0.00004462264,0.0000062974805,7.639033e-7,0.0000016209044,0.00004767005,0.000006041915,0.00012918776],"genre_scores_gemma":[0.9997905,0.000006224933,0.000065461194,0.0000035193555,0.0000013290213,0.0000013276849,0.00008613842,0.0000012088364,0.00004429685],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999504,0.0000042449697,0.0000027922094,0.000015971626,0.0000102393815,0.000016395068],"domain_scores_gemma":[0.9998265,0.000013098817,0.00007024534,0.000015511116,0.000018245666,0.00005650145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000100217265,0.00013976822,0.00016626914,0.00036433764,0.0003534462,0.00022397815,0.00018290315,0.00019813639,0.00047352628],"category_scores_gemma":[0.00026440315,0.000090130976,0.00012148592,0.00026159704,0.00018109473,0.000112975315,0.00033162336,0.00021584815,0.00009549147],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015627219,0.000053579555,0.8954954,0.000014491688,0.000040419985,0.0012062641,0.00047959932,0.0004744741,0.09608469,0.00009969394,0.00021223526,0.005682758],"study_design_scores_gemma":[0.0000017578654,0.000025848596,0.99883837,7.583817e-7,0.0000043484274,0.00013102661,0.000051218067,0.0002710777,0.00056462677,0.000013515923,0.00009556173,0.0000019217466],"about_ca_topic_score_codex":0.00597468,"about_ca_topic_score_gemma":0.010415778,"teacher_disagreement_score":0.00597468,"about_ca_system_score_codex":0.0002865545,"about_ca_system_score_gemma":0.00010292698,"threshold_uncertainty_score":0.011879802},"labels":[],"label_agreement":null},{"id":"W3126033875","doi":"10.3847/1538-4357/abe6ac","title":"Toward Cosmological Simulations of Dark Matter on Quantum Computers","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Quantum Computing Algorithms and Architecture","field":"Computer Science","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"National Aeronautics and Space Administration","keywords":"Dark energy; Physics; Dark matter; Quantum; Quantum computer; Statistical physics; Nonlinear system; Universe; Theoretical physics; Quantum algorithm; Classical mechanics; Quantum mechanics; Astrophysics; Cosmology","score_opus":0.01817902928475516,"score_gpt":0.2465043384994797,"score_spread":0.22832530921472455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3126033875","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.37748334,0.00036949146,0.58748317,0.0030658322,0.00021997854,0.00017114228,0.000095899995,0.0008760048,0.030235164],"genre_scores_gemma":[0.8435304,0.00019634468,0.15256089,0.00025045275,0.000046754136,0.00012224649,0.00005668316,0.000118011514,0.0031181674],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99973756,0.00014005073,0.0000062712525,0.00001778044,0.00007066572,0.00002762316],"domain_scores_gemma":[0.999151,0.00049372856,0.00004108625,0.00009217926,0.00012808945,0.000093960225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010530986,0.00030439848,0.0004911873,0.00034726883,0.0006380496,0.00095417467,0.0011030067,0.0011486055,0.0029017378],"category_scores_gemma":[0.0031449131,0.00029711425,0.00034465714,0.0002956931,0.0016260891,0.0012956811,0.0012539822,0.0012234971,0.00029289827],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009242481,0.00009703781,0.0008044118,0.000059029426,0.000024956355,0.000067929104,0.00012654655,0.63586724,0.0055819387,0.35121697,0.0010424044,0.005019152],"study_design_scores_gemma":[0.000011901693,0.00000603298,0.000035615758,0.0000027131043,0.0000011147138,0.0000031565323,0.0000056561753,0.9758203,0.00040539665,0.02330561,0.0004000402,0.0000024259234],"about_ca_topic_score_codex":0.0038334099,"about_ca_topic_score_gemma":0.0025448739,"teacher_disagreement_score":0.0038334099,"about_ca_system_score_codex":0.000911596,"about_ca_system_score_gemma":0.0009762248,"threshold_uncertainty_score":0.009707272},"labels":[],"label_agreement":null},{"id":"W3126318718","doi":"10.3847/1538-4357/abe59f","title":"ALMA Observations of the Asymmetric Dust Disk around DM Tau","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Radiative transfer; Spectral energy distribution; Sublimation (psychology); Submillimeter Array; Millimeter; Planet; Monte Carlo method; Cosmic dust; Angular resolution (graph drawing)","score_opus":0.022652882674847438,"score_gpt":0.24429831371023894,"score_spread":0.2216454310353915,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3126318718","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99795914,0.000087809996,0.0005883428,0.000023537224,0.000005224873,0.000005240123,0.00025387204,0.000050075116,0.0010268473],"genre_scores_gemma":[0.9987232,0.000025123976,0.0008426947,0.000010430768,0.000012590467,0.0000036740178,0.00024274121,0.000005770293,0.00013366711],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999347,0.000009022234,0.0000021205667,0.000021231255,0.000019810157,0.0000131780225],"domain_scores_gemma":[0.9998568,0.000027184402,0.00003552043,0.000022606058,0.00002387826,0.0000339736],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014989727,0.00018330802,0.00017655513,0.00050517987,0.00036209766,0.00030946452,0.00028080255,0.00022975588,0.00059032993],"category_scores_gemma":[0.00030496606,0.00013149166,0.00024932282,0.0002544345,0.000118861164,0.00019367134,0.00022001819,0.00026270378,0.00016503617],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086008525,0.0002248725,0.57217133,0.00007746868,0.00021673772,0.0012155629,0.00053449353,0.007926575,0.39451092,0.0008866556,0.0009870984,0.020388143],"study_design_scores_gemma":[0.00006170407,0.00023161777,0.9646395,0.000008453977,0.00006913811,0.00037771405,0.00009832486,0.02061745,0.011081055,0.00019845128,0.0026037078,0.000012973134],"about_ca_topic_score_codex":0.0027352923,"about_ca_topic_score_gemma":0.0035487434,"teacher_disagreement_score":0.0027352923,"about_ca_system_score_codex":0.00036239775,"about_ca_system_score_gemma":0.000089498826,"threshold_uncertainty_score":0.0054388046},"labels":[],"label_agreement":null},{"id":"W3126869682","doi":"10.3847/1538-4357/abe94a","title":"How Does the Polar Dust Affect the Correlation between Dust Covering Factor and Eddington Ratio in Type 1 Quasars Selected from the Sloan Digital Sky Survey Data Release 16?","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Japan Society for the Promotion of Science; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; Max-Planck-Institut für Astrophysik; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Torus; Quasar; Luminosity; Polar; Sky; Active galactic nucleus; Radiative transfer; Infrared","score_opus":0.01798786273364766,"score_gpt":0.22766383745098,"score_spread":0.20967597471733235,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3126869682","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998844,0.000093769355,0.00011104241,0.000017989041,0.000002446268,0.0000014312388,0.00063125376,0.000007042709,0.0002908705],"genre_scores_gemma":[0.9989146,0.00002712428,0.000041225976,0.000004301876,0.000005249969,0.0000011130195,0.00091073837,0.0000024640417,0.00009329117],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997168,0.000047377544,0.000029959567,0.00008366786,0.000057531495,0.000064624655],"domain_scores_gemma":[0.9976191,0.00047285366,0.0010845241,0.00023565663,0.00029714796,0.00029075381],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049822114,0.00022921104,0.00021040044,0.0012047815,0.00022066443,0.0007070946,0.00021901939,0.00021509704,0.0012370422],"category_scores_gemma":[0.0016115851,0.000117833435,0.0003245191,0.00090360903,0.00024440495,0.00032933758,0.0002852736,0.00015742125,0.00025998484],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000010178119,0.00000263523,0.9991492,0.0000023682749,0.000022209759,0.000017284627,0.000012939132,0.00012744818,0.00016984332,0.000008092531,0.000048736678,0.00042900917],"study_design_scores_gemma":[4.4943013e-7,0.000003943474,0.99940944,0.0000010925887,0.0000069969806,0.000018220131,0.000031560747,0.0003926665,0.0000563494,0.000007864688,0.00007046693,0.0000010595957],"about_ca_topic_score_codex":0.0098801255,"about_ca_topic_score_gemma":0.012746179,"teacher_disagreement_score":0.0098801255,"about_ca_system_score_codex":0.00021464059,"about_ca_system_score_gemma":0.00012543735,"threshold_uncertainty_score":0.019645214},"labels":[],"label_agreement":null},{"id":"W3127589372","doi":"10.3847/1538-4357/ac0e91","title":"Detecting Neutrino Mass by Combining Matter Clustering, Halos, and Voids","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Physics; Neutrino; Omega; Halo; Matter power spectrum; Particle physics; Baryon; Halo mass function; Spectral density; Astrophysics; Sigma; Dark matter; Galaxy; Statistics; Redshift; Quantum mechanics; Mathematics","score_opus":0.0062915014217234805,"score_gpt":0.20804640836452126,"score_spread":0.2017549069427978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3127589372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9704564,0.000067386245,0.02767741,0.00008277021,0.0000056644735,0.000010722795,0.00023927593,0.00033678632,0.00112357],"genre_scores_gemma":[0.99155176,0.000018416738,0.008135934,0.000014669066,0.0000045736074,0.0000042432243,0.00012748102,0.000031051986,0.00011180618],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997379,0.000117724325,0.000007862714,0.00004508346,0.00006550952,0.000025905158],"domain_scores_gemma":[0.9980836,0.0011313667,0.00034010728,0.00018601965,0.00013077648,0.00012806726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014165672,0.00046675839,0.0004195495,0.0012472924,0.000250973,0.0008377802,0.0004771136,0.00047525682,0.000794777],"category_scores_gemma":[0.004520569,0.0004753785,0.00041943934,0.0008035532,0.0004861435,0.000753871,0.00085965963,0.00030284346,0.00012248907],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011070522,0.00017114855,0.2797856,0.00011652777,0.00044864684,0.00022221514,0.00026597345,0.59920305,0.06762186,0.013587036,0.0007147326,0.036756206],"study_design_scores_gemma":[0.000028040731,0.00006072698,0.040928576,0.000011582112,0.000041534575,0.00005225904,0.00003475404,0.9407195,0.00979526,0.007978184,0.00029772404,0.000051919953],"about_ca_topic_score_codex":0.0034923956,"about_ca_topic_score_gemma":0.0044880756,"teacher_disagreement_score":0.0034923956,"about_ca_system_score_codex":0.00037300092,"about_ca_system_score_gemma":0.0003413891,"threshold_uncertainty_score":0.0074915886},"labels":[],"label_agreement":null},{"id":"W3127816455","doi":"10.3847/1538-4357/abe2a5","title":"SDSS-IV MaNGA: The Radial Profile of Enhanced Star Formation in Close Galaxy Pairs","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Galaxy; Stellar mass; Star formation; Effective radius; Redshift; RADIUS; Astronomy","score_opus":0.0069110615787278395,"score_gpt":0.21032928255895497,"score_spread":0.20341822098022713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3127816455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99925154,0.000044412016,0.000062973624,0.000006769689,8.866335e-7,0.000002006094,0.00029057264,0.000009793658,0.0003310873],"genre_scores_gemma":[0.99948597,0.000009812955,0.00007268003,0.0000025383838,0.0000014346151,0.0000015307706,0.00034853423,0.000002267045,0.000075161115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997658,0.00005326909,0.000013805826,0.000076156866,0.000046888108,0.00004404848],"domain_scores_gemma":[0.99874485,0.00015421047,0.0004552256,0.00013083467,0.00014405973,0.00037069488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003481544,0.00016665802,0.0002739846,0.0016000629,0.00030975707,0.00038941507,0.00016632829,0.00016712732,0.0009774491],"category_scores_gemma":[0.0012440877,0.00010917182,0.00018630445,0.00080966984,0.00020819988,0.00021444503,0.0006644587,0.0001290503,0.00034286547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007772231,0.00001346262,0.99441177,0.000007344645,0.000027801687,0.000057506808,0.00014457114,0.00011308594,0.003165882,0.000044302156,0.0000905479,0.00184594],"study_design_scores_gemma":[7.033169e-7,0.000013181289,0.99952555,8.6926843e-7,0.0000030866659,0.000060915092,0.00005264015,0.0001216902,0.00013639266,0.000010713747,0.00007311289,0.0000011199074],"about_ca_topic_score_codex":0.0039662654,"about_ca_topic_score_gemma":0.004904826,"teacher_disagreement_score":0.0039662654,"about_ca_system_score_codex":0.00021670392,"about_ca_system_score_gemma":0.000084021834,"threshold_uncertainty_score":0.00788635},"labels":[],"label_agreement":null},{"id":"W3127869776","doi":"10.3847/1538-4357/ac2b33","title":"FIRST J153350.8+272729: The Radio Afterglow of a Decades-old Tidal Disruption Event","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Smithsonian Astrophysical Observatory; Goddard Space Flight Center; Jet Propulsion Laboratory; University of Toronto; University of Utah; Astrophysics Division; Canadian Institute for Advanced Research; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Alfred P. Sloan Foundation; Astrophysics Science Division; Office of Science; Canada Research Chairs; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Luminosity; Afterglow; Astrophysics; Galaxy; Redshift; Astronomy; Radio telescope; Event (particle physics); X-shaped radio galaxy; Radio galaxy; Gamma-ray burst","score_opus":0.008380428921439791,"score_gpt":0.22865416907107297,"score_spread":0.2202737401496332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3127869776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99619186,0.00046567983,0.0005415485,0.00014271407,0.000035337445,0.000009698403,0.0002997462,0.00005022263,0.0022631253],"genre_scores_gemma":[0.9984816,0.00009190646,0.00031629705,0.000078054996,0.000027870514,0.0000036163306,0.00045962393,0.000010549782,0.0005305449],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999286,0.0000031585287,0.0000029423632,0.000029196031,0.000012904819,0.000023174574],"domain_scores_gemma":[0.9997092,0.000020076952,0.00009644955,0.000038928727,0.000031004765,0.000104414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016115147,0.00025795083,0.0003480643,0.00054753956,0.000511273,0.0005885218,0.0004092658,0.00041582444,0.0013764341],"category_scores_gemma":[0.00023707924,0.00012548281,0.00020742079,0.00045879086,0.00038052446,0.00021978148,0.0006747228,0.00038613574,0.0005919927],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009154071,0.00020906678,0.63417083,0.0002069322,0.00021273269,0.028791174,0.00078664464,0.0012015953,0.28948495,0.0029723127,0.004211848,0.03683661],"study_design_scores_gemma":[0.000045527744,0.00027802208,0.96140814,0.00003716281,0.000089821326,0.010779402,0.0004428974,0.0014487922,0.008680948,0.0008521519,0.015895354,0.00004190462],"about_ca_topic_score_codex":0.0022965535,"about_ca_topic_score_gemma":0.0029886786,"teacher_disagreement_score":0.0022965535,"about_ca_system_score_codex":0.0005011614,"about_ca_system_score_gemma":0.00015927842,"threshold_uncertainty_score":0.004604578},"labels":[],"label_agreement":null},{"id":"W3128431752","doi":"10.3847/1538-4357/abe306","title":"A Massive, Clumpy Molecular Gas Distribution and Displaced AGN in Zw 3146","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; University of Manitoba","funders":"Science and Technology Facilities Council","keywords":"Galaxy; Galaxy cluster; Gravitational potential; Cluster (spacecraft); Brightest cluster galaxy; Gravitation; Molecular cloud; Intracluster medium; Gravitational lens","score_opus":0.004025316421965663,"score_gpt":0.2037886215090624,"score_spread":0.19976330508709675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3128431752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99948055,0.0000442369,0.00008399982,0.000019227647,0.0000015526634,0.0000021081794,0.0001223116,0.000005977867,0.00024001842],"genre_scores_gemma":[0.9994929,0.0000172356,0.00011386796,0.000008150743,0.0000040684263,0.0000012311685,0.00015302835,0.0000021303767,0.00020747668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999372,0.000003628333,0.0000032738583,0.00001716194,0.000018929839,0.000019855752],"domain_scores_gemma":[0.9998005,0.00000940756,0.000092942755,0.000015333706,0.000018689017,0.00006309801],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000085433065,0.00015533227,0.00018538971,0.000814324,0.00039713038,0.0003812303,0.00027949645,0.00023469751,0.0016464172],"category_scores_gemma":[0.00020545696,0.00011097525,0.00012337646,0.0005427662,0.00030095415,0.00017553607,0.00042381868,0.00021495373,0.00019538963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033335798,0.000058464735,0.908244,0.000020138194,0.000040286322,0.002100223,0.00035949773,0.00022318569,0.08168871,0.00027555262,0.0002910613,0.0063655744],"study_design_scores_gemma":[0.000004104794,0.00002614138,0.99808455,0.0000018992929,0.000004713715,0.0006052423,0.0000875724,0.00014790284,0.00068283745,0.00006088293,0.0002918665,0.0000023969505],"about_ca_topic_score_codex":0.0056625498,"about_ca_topic_score_gemma":0.008813117,"teacher_disagreement_score":0.0056625498,"about_ca_system_score_codex":0.00032338654,"about_ca_system_score_gemma":0.000075683805,"threshold_uncertainty_score":0.011259198},"labels":[],"label_agreement":null},{"id":"W3128671874","doi":"10.3847/1538-4357/abe37f","title":"On the Observational Difference between the Accretion Disk–Corona Connections among Super- and Sub-Eddington Accreting Active Galactic Nuclei","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Active galactic nucleus; Accretion (finance); Accretion disc; Monochromatic color; Luminosity; Black hole (networking); Photon","score_opus":0.029033870293736292,"score_gpt":0.24712169005525692,"score_spread":0.2180878197615206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3128671874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99968994,0.000049745355,0.00004562649,0.0000017087716,2.769023e-7,8.578774e-7,0.000061042876,0.0000011422925,0.0001497351],"genre_scores_gemma":[0.9997327,0.000025063222,0.000041073803,0.0000024468802,0.0000012317458,0.0000010257043,0.00013702802,6.877262e-7,0.00005887749],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981254,0.000045765708,0.00002047837,0.000059396672,0.000034594166,0.000027284801],"domain_scores_gemma":[0.9984296,0.0004322513,0.00064461696,0.00017009141,0.00015056609,0.00017286457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041838508,0.0001613143,0.00013678138,0.0011185511,0.00020292775,0.00043744218,0.00023763097,0.00014328802,0.0010161158],"category_scores_gemma":[0.0014198594,0.00012988671,0.00014325755,0.00050432177,0.00031909894,0.0002640915,0.00045212102,0.00011954441,0.00025367682],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036852973,0.000006448796,0.9967715,0.0000031763993,0.000014046068,0.000022198043,0.000050009654,0.000022623257,0.0020515663,0.000010006014,0.000006610469,0.0010048813],"study_design_scores_gemma":[4.4035758e-7,0.000016186985,0.9996049,9.545264e-7,0.000004746537,0.000073457464,0.000036326783,0.00003705489,0.00018642581,0.0000054943453,0.000033643915,4.5203635e-7],"about_ca_topic_score_codex":0.0012556082,"about_ca_topic_score_gemma":0.0020880806,"teacher_disagreement_score":0.0012556082,"about_ca_system_score_codex":0.00011722309,"about_ca_system_score_gemma":0.00006833484,"threshold_uncertainty_score":0.003399253},"labels":[],"label_agreement":null},{"id":"W3128799051","doi":"10.3847/1538-4357/abe40b","title":"Discovery of Beryllium in White Dwarfs Polluted by Planetesimal Accretion","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"White dwarf; Beryllium; Planetesimal; Accretion (finance); Spectral line; Spallation; Meteorite; Heavy element","score_opus":0.005194668333746494,"score_gpt":0.19994956283996354,"score_spread":0.19475489450621705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3128799051","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990245,0.00014334811,0.00021113212,0.00001197366,0.0000070138235,0.0000024860863,0.00009226732,0.000015067627,0.00049204944],"genre_scores_gemma":[0.99866223,0.00005988376,0.0001922251,0.000017516328,0.0000056017057,0.000001722521,0.00018575245,0.000010843221,0.00086420984],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998647,0.000012777204,0.000008167176,0.00004204902,0.000040884865,0.000031404576],"domain_scores_gemma":[0.9996743,0.00004950034,0.00007238594,0.000028164235,0.00008242904,0.00009326842],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020378691,0.00028646737,0.0003529687,0.0009923554,0.00081321003,0.00076948036,0.00020721876,0.00037436478,0.0009909006],"category_scores_gemma":[0.00048637218,0.0001844021,0.00012524099,0.00044961792,0.00045644052,0.00021962229,0.00051073404,0.00016914605,0.0003129137],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009630619,0.00006498139,0.1942169,0.00007126329,0.00008366133,0.0018415889,0.0009183144,0.00008569286,0.7967749,0.0002008731,0.00015597547,0.0046228115],"study_design_scores_gemma":[0.000018048659,0.00046172587,0.86042804,0.000011022323,0.00005510058,0.0024988863,0.0005586153,0.0005102981,0.13195886,0.00018523257,0.003303197,0.000011063416],"about_ca_topic_score_codex":0.0027350269,"about_ca_topic_score_gemma":0.002251572,"teacher_disagreement_score":0.0027350269,"about_ca_system_score_codex":0.00027156726,"about_ca_system_score_gemma":0.00014081875,"threshold_uncertainty_score":0.0054382086},"labels":[],"label_agreement":null},{"id":"W3129708769","doi":"10.3847/1538-4357/abe30a","title":"Erratum: “A Partial Inventory of Observational Anisotropies in Single-dish Line-intensity Mapping” (2019, ApJ, 881, 149)","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Medical Imaging Techniques and Applications","field":"Medicine","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Intensity (physics); Line (geometry); Astrophysics; Observational study; Astronomy; Optics; Medicine; Geometry","score_opus":0.06585871044836662,"score_gpt":0.3030123753083138,"score_spread":0.2371536648599472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3129708769","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00065776106,0.001460486,0.00095589826,0.05708654,0.92431533,0.000026370528,0.0034306922,0.0006378991,0.011429034],"genre_scores_gemma":[0.020623937,0.0072820466,0.011413932,0.1407764,0.34630024,0.0002006408,0.0133142015,0.0042919805,0.4557967],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9978951,0.00020888758,0.00035348395,0.00030394815,0.0010987249,0.00013991985],"domain_scores_gemma":[0.98549867,0.00357824,0.00090682076,0.001261616,0.007910673,0.0008440263],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025103302,0.0018185403,0.001058329,0.0035236164,0.0042925593,0.0032905734,0.002342623,0.0042153257,0.048085954],"category_scores_gemma":[0.026433619,0.00081255275,0.0010684065,0.0021554488,0.0017628822,0.0028518874,0.0019032999,0.007923456,0.037522644],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030104242,0.0000062982813,0.00010762827,0.000038640566,0.000005112069,0.00011296128,0.000014110704,0.000024390158,0.00012918336,0.00042105012,0.9957247,0.0033858118],"study_design_scores_gemma":[0.000025010144,0.000020916197,0.0023969917,0.00017646536,0.000035539022,0.00040354434,0.000120896235,0.00023933439,0.00076811784,0.0020358036,0.9937251,0.00005230493],"about_ca_topic_score_codex":0.022668032,"about_ca_topic_score_gemma":0.038544487,"teacher_disagreement_score":0.048085954,"about_ca_system_score_codex":0.0031725229,"about_ca_system_score_gemma":0.0035373801,"threshold_uncertainty_score":0.16086358},"labels":[],"label_agreement":null},{"id":"W3130342124","doi":"10.3847/1538-4357/ac222d","title":"The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: A Case Study on GW190425","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":61,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; U.S. Department of Energy; Nuclear Safety and Security Commission; University of Alberta; Vetenskapsrådet; National Science Foundation","keywords":"Physics; Kilonova; Neutron star; Gravitational wave; Astrophysics; Astronomy; Light curve; Binary number; Black hole (networking); r-process; Pulsar; Nucleosynthesis; LIGO; Supernova","score_opus":0.06898454423777392,"score_gpt":0.4169056150903727,"score_spread":0.3479210708525988,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3130342124","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.941028,0.00073063903,0.0490787,0.0028159283,0.00003063516,0.00004082019,0.00033444742,0.00014534614,0.005795453],"genre_scores_gemma":[0.97900635,0.0001732095,0.019772626,0.000113647635,0.000047543886,0.000010809016,0.00020118288,0.000058098754,0.00061666354],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990694,0.00044905432,0.000053287495,0.00012764915,0.00022463028,0.00007604535],"domain_scores_gemma":[0.9933594,0.0044566784,0.00059477374,0.0007530111,0.00049949164,0.0003366452],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004972306,0.00037300432,0.00051643763,0.0018023811,0.0008270296,0.0017725965,0.0007080771,0.00094193907,0.0012876494],"category_scores_gemma":[0.008903756,0.0002079854,0.0004583384,0.0013023148,0.0009905678,0.0014304523,0.0020109995,0.0009368847,0.000161398],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039973145,0.0002486341,0.6954963,0.0001873216,0.0002690856,0.018973144,0.0019866426,0.04897468,0.009862451,0.06274345,0.0033988194,0.15745969],"study_design_scores_gemma":[0.000070813105,0.000306148,0.54699165,0.00021526054,0.00013038157,0.012549419,0.0043894574,0.2578696,0.010344244,0.14117403,0.025789807,0.00016915904],"about_ca_topic_score_codex":0.0049408446,"about_ca_topic_score_gemma":0.007638952,"teacher_disagreement_score":0.004972306,"about_ca_system_score_codex":0.0007464347,"about_ca_system_score_gemma":0.00045373404,"threshold_uncertainty_score":0.026296377},"labels":[],"label_agreement":null},{"id":"W3130795358","doi":"10.3847/1538-4357/abfaf9","title":"On the Evolution of Supermassive Primordial Stars in Cosmological Flows","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Supermassive black hole; Halo; Accretion (finance); Stars; Radiative transfer; Stellar evolution","score_opus":0.008437617442571524,"score_gpt":0.2091589656438176,"score_spread":0.2007213482012461,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3130795358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969092,0.00009396261,0.001306015,0.00007656633,0.000003906505,0.0000048590446,0.000087871085,0.000033283024,0.001484304],"genre_scores_gemma":[0.9993351,0.000042552536,0.00034897667,0.000011253298,0.000003111653,0.0000021526942,0.000040925726,0.000007661549,0.00020825464],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994636,0.000018322175,0.0000022029499,0.0000115749845,0.0000071436725,0.000014409189],"domain_scores_gemma":[0.99937975,0.00020716574,0.00018347513,0.000032792013,0.000031073363,0.00016575109],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003670466,0.00035342984,0.0003324261,0.0005768767,0.00047844704,0.0010517867,0.00048075072,0.0007051942,0.0015274966],"category_scores_gemma":[0.0015137243,0.0002651097,0.0003114298,0.00033842324,0.0006754562,0.00071256346,0.0007655998,0.0003745049,0.00019905916],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032530303,0.00022146016,0.34156725,0.00008030005,0.00010304146,0.0009170515,0.0005052943,0.5891475,0.019216899,0.03878643,0.00093970617,0.008189762],"study_design_scores_gemma":[0.000053848355,0.000095253396,0.11456958,0.00001954841,0.000032643708,0.00014559217,0.00014612536,0.8735595,0.0017334928,0.008810319,0.00080137886,0.000032844753],"about_ca_topic_score_codex":0.005601135,"about_ca_topic_score_gemma":0.0028368388,"teacher_disagreement_score":0.005601135,"about_ca_system_score_codex":0.0011179263,"about_ca_system_score_gemma":0.0002989957,"threshold_uncertainty_score":0.011137068},"labels":[],"label_agreement":null},{"id":"W3132181818","doi":"10.3847/1538-4357/abe532","title":"The Galactic H ii Region Luminosity Function at Radio and Infrared Wavelengths","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Science Foundation","keywords":"Milky Way; Stars; Infrared; Spiral galaxy; Luminosity; Wavelength; Luminosity function; Star formation; Spectral index","score_opus":0.010230492505612178,"score_gpt":0.20378641352569773,"score_spread":0.19355592102008556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3132181818","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947649,0.0001084968,0.0010146484,0.000022041666,0.0000032879857,0.0000052573087,0.0020713538,0.00006333556,0.0019466762],"genre_scores_gemma":[0.9970497,0.00004109191,0.00039883424,0.000013907187,0.0000086219525,0.0000060542284,0.0021648929,0.000015218936,0.00030158836],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978274,0.000045526795,0.000013936906,0.00005886781,0.000057937516,0.00004098133],"domain_scores_gemma":[0.99878794,0.0003653825,0.0003865647,0.00014006108,0.00017694019,0.00014312322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005863791,0.00026170854,0.00027514712,0.0017869388,0.00015226094,0.0007997047,0.00029718736,0.00024730407,0.0027446053],"category_scores_gemma":[0.001896613,0.000119378,0.00031564024,0.0010997893,0.00018615369,0.00052618334,0.0002741696,0.00017286751,0.0013440326],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036032612,0.00001708836,0.9929987,0.000007904966,0.00007779654,0.000019610183,0.000029318988,0.0013645635,0.0014759627,0.000095878815,0.0002773679,0.0035996863],"study_design_scores_gemma":[0.000001946389,0.000019349169,0.99705887,0.0000027902277,0.000012635094,0.000037101632,0.00007070542,0.0020393867,0.00042029453,0.000082626124,0.00025105,0.0000032785426],"about_ca_topic_score_codex":0.0034948871,"about_ca_topic_score_gemma":0.0019801878,"teacher_disagreement_score":0.0034948871,"about_ca_system_score_codex":0.00025790065,"about_ca_system_score_gemma":0.00006485916,"threshold_uncertainty_score":0.009181678},"labels":[],"label_agreement":null},{"id":"W3133086882","doi":"10.3847/1538-4357/abe711","title":"The Planck Submillimeter Properties of Galactic High-mass Star-forming Regions: Dust Temperatures, Luminosities, Masses, and Star Formation Efficiency","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"","keywords":"Physics; Astrophysics; Star formation; Luminosity; Molecular cloud; RADIUS; Planck; Young stellar object; Astronomy; Galaxy; Stars","score_opus":0.012993717300303223,"score_gpt":0.21185969801604795,"score_spread":0.19886598071574474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3133086882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99392444,0.00015961642,0.0004710032,0.0000149512725,0.0000017646086,0.000003438494,0.003951541,0.000048349448,0.001424933],"genre_scores_gemma":[0.9972699,0.00005322846,0.00032520085,0.0000055972896,0.0000040813798,0.0000034688137,0.0021683725,0.0000062981494,0.00016383281],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991035,0.000012642334,0.00000748455,0.000030722993,0.000020027595,0.000018708086],"domain_scores_gemma":[0.99930286,0.00018858866,0.00026882673,0.0000890247,0.000060626724,0.000089975634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024153775,0.0001825096,0.00015381914,0.0010640576,0.0001243102,0.0004483596,0.00015937108,0.000172451,0.0023068367],"category_scores_gemma":[0.0008455132,0.00012140764,0.00020622123,0.0010124501,0.00012209098,0.0003222346,0.00027844083,0.00012334328,0.00064933236],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004115917,0.00001114054,0.99114436,0.000018743976,0.00006938875,0.000031704076,0.000067182205,0.00088326744,0.0034509038,0.0001093933,0.00025548527,0.003917168],"study_design_scores_gemma":[4.7150047e-7,0.0000038043204,0.99885046,0.0000010741462,0.0000063202287,0.00003764511,0.000022598473,0.0003994273,0.00048807956,0.000022860193,0.00016566961,0.000001576577],"about_ca_topic_score_codex":0.001775607,"about_ca_topic_score_gemma":0.0012802382,"teacher_disagreement_score":0.0023068367,"about_ca_system_score_codex":0.00012460025,"about_ca_system_score_gemma":0.00005012847,"threshold_uncertainty_score":0.007717192},"labels":[],"label_agreement":null},{"id":"W3133305186","doi":"10.3847/1538-4357/abe401","title":"The Physical Drivers of the Luminosity-weighted Dust Temperatures in High-redshift Galaxies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Star formation; Sigma; Lambda; Luminosity; Equivalent width; Spectral line; Astronomy; Emission spectrum","score_opus":0.004634611575334248,"score_gpt":0.19900054578233117,"score_spread":0.19436593420699694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3133305186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993519,0.00005399619,0.00013891055,0.000020015721,8.362742e-7,0.0000010502952,0.000082029714,0.0000077133345,0.00034341973],"genre_scores_gemma":[0.99986196,0.000008463237,0.000026681026,0.0000035814073,0.0000020567252,4.240182e-7,0.00004830766,0.0000011601907,0.000047446458],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999813,0.000025911402,0.000011657218,0.00006394044,0.000042085685,0.00004343459],"domain_scores_gemma":[0.9986041,0.00028747905,0.00058593956,0.00015873284,0.00015222086,0.00021154441],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003298032,0.00015893811,0.00020832637,0.0010630753,0.00025426788,0.001123322,0.00032842578,0.00034966253,0.0018288784],"category_scores_gemma":[0.0011455815,0.0001854813,0.00020062295,0.0006997195,0.0006749401,0.00046555576,0.00043301127,0.00025934164,0.0003598639],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022103126,0.000011560568,0.9938221,0.0000046609775,0.000029070416,0.000029823132,0.00014368021,0.00018737465,0.0045128204,0.00019397632,0.000054319855,0.0009883414],"study_design_scores_gemma":[6.868368e-7,0.0000037336704,0.9995983,6.1235636e-7,0.0000017948068,0.00001650587,0.000054538898,0.00014299285,0.00009686885,0.00005398437,0.000029120662,8.6378407e-7],"about_ca_topic_score_codex":0.003595259,"about_ca_topic_score_gemma":0.004146039,"teacher_disagreement_score":0.003595259,"about_ca_system_score_codex":0.00038804853,"about_ca_system_score_gemma":0.0000767637,"threshold_uncertainty_score":0.007148683},"labels":[],"label_agreement":null},{"id":"W3133892305","doi":"10.3847/1538-4357/ac06a3","title":"Detection of Galactic and Extragalactic Millimeter-wavelength Transient Sources with SPT-3G","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Three-Speed Logic (Canada); Canadian Institute for Advanced Research; McGill University","funders":"Fermilab; High Energy Physics; Australian Research Council; Science and Technology Facilities Council; Science Mission Directorate; University of California, Los Angeles; McGill University; University of Chicago; Jet Propulsion Laboratory; Centre National d’Etudes Spatiales; Argonne National Laboratory; California Institute of Technology; U.S. Department of Energy; Gordon and Betty Moore Foundation; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; Office of Science; National Science Foundation; European Space Agency; National Aeronautics and Space Administration","keywords":"Telescope; Stars; Population; Variable star; Transient (computer programming); Cosmic microwave background; Millimeter; Angular resolution (graph drawing)","score_opus":0.006789086092980295,"score_gpt":0.19111816960034086,"score_spread":0.18432908350736057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3133892305","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99596053,0.00008852309,0.0010776665,0.000058364123,0.000008296405,0.00001661134,0.0011546303,0.00010517321,0.0015302072],"genre_scores_gemma":[0.9958473,0.000038574555,0.0017369762,0.00006632734,0.000015484962,0.00001319773,0.0020036146,0.000018406812,0.00026024607],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997985,0.000020195623,0.000009377661,0.000056419096,0.000066304136,0.000049206985],"domain_scores_gemma":[0.99903536,0.00010536529,0.00040186621,0.00011623078,0.00012775685,0.00021346862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035262192,0.00022595667,0.00026547138,0.0012004314,0.00028002216,0.0005963936,0.00029998878,0.00047579355,0.0011590447],"category_scores_gemma":[0.00052833103,0.00018037079,0.00029850067,0.001257864,0.0002494379,0.00034241355,0.00060030544,0.00042841752,0.00032997807],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029654187,0.00008625943,0.91191065,0.00004782662,0.00011249943,0.00053660956,0.00025684616,0.00036322812,0.07139212,0.00016864136,0.0011593559,0.0136693735],"study_design_scores_gemma":[0.000009133995,0.00007289118,0.99571556,0.0000030944097,0.000020704798,0.0002967544,0.000040364892,0.00047459724,0.0026913586,0.000042323914,0.0006294117,0.0000037784569],"about_ca_topic_score_codex":0.0019261321,"about_ca_topic_score_gemma":0.004891954,"teacher_disagreement_score":0.0019261321,"about_ca_system_score_codex":0.00023895373,"about_ca_system_score_gemma":0.0001602294,"threshold_uncertainty_score":0.0038774014},"labels":[],"label_agreement":null},{"id":"W3134185226","doi":"10.3847/1538-4357/abeb17","title":"Probing the Disk–Corona Systems and Broad-line Regions of Changing-look Quasars with X-Ray and Optical Observations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Quasar; Accretion (finance); Emission spectrum; Active galactic nucleus; Spectral line; Eddington luminosity; Accretion disc","score_opus":0.01622115864929237,"score_gpt":0.21431619600794588,"score_spread":0.19809503735865353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3134185226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951794,0.00018981405,0.0006595374,0.000058455716,0.0000051373104,0.000012036519,0.0007218621,0.00005378372,0.0031199644],"genre_scores_gemma":[0.9971386,0.00006923113,0.0013940538,0.00008843244,0.000011454921,0.000007435329,0.0006244314,0.000013362944,0.00065309176],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998996,0.000014043905,0.0000057516586,0.000028118055,0.000019411129,0.00003309668],"domain_scores_gemma":[0.9996393,0.000038325248,0.00011705927,0.000035519915,0.000057744368,0.00011207572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027768896,0.00014365945,0.00011879918,0.0008551955,0.00021963587,0.00056785886,0.0002215697,0.00025087205,0.0028498839],"category_scores_gemma":[0.0003236916,0.00015489741,0.00014617934,0.00044355216,0.0001768962,0.00042801013,0.00036477137,0.00023412333,0.0005565409],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017072626,0.00008557803,0.92172337,0.000028640925,0.00006318481,0.00024390357,0.00022696165,0.000120194956,0.06213401,0.00014811469,0.0010596467,0.01399559],"study_design_scores_gemma":[0.000002812862,0.000030651558,0.9971071,0.0000026351338,0.000008909341,0.00015132806,0.00012658726,0.00015601741,0.0017463859,0.000035096138,0.00062951515,0.0000029285366],"about_ca_topic_score_codex":0.0022415665,"about_ca_topic_score_gemma":0.004960044,"teacher_disagreement_score":0.0028498839,"about_ca_system_score_codex":0.00015993069,"about_ca_system_score_gemma":0.000044734836,"threshold_uncertainty_score":0.009533763},"labels":[],"label_agreement":null},{"id":"W3134312677","doi":"10.3847/1538-4357/abfe5f","title":"Fast Dissipation of Colliding Alfvén Waves in a Magnetically Dominated Plasma","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute","funders":"Natural Sciences and Engineering Research Council of Canada; Ministry of Colleges and Universities; Nuclear Safety and Security Commission; Compute Canada; National Aeronautics and Space Administration; U.S. Department of Energy; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada; Government of Canada; National Science Foundation","keywords":"Physics; Current sheet; Dissipation; Magnetohydrodynamics; Magnetic field; Instability; Astrophysics; Magnetic reconnection; Magnetar; Plasma; Magnetic energy; Kink instability; Computational physics; Pulsar; Mechanics; Magnetization","score_opus":0.004940952362406175,"score_gpt":0.21689366884555103,"score_spread":0.21195271648314484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3134312677","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99564457,0.000060783863,0.0017499302,0.00014888989,0.000020475394,0.0000155505,0.00005739636,0.00008948326,0.002212887],"genre_scores_gemma":[0.9991743,0.00002149319,0.0004886708,0.000022420514,0.000006327821,0.0000109272705,0.000044129185,0.000014209357,0.00021749752],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988115,0.000021685937,0.0000046911837,0.000012605822,0.000021111,0.000058742815],"domain_scores_gemma":[0.99967885,0.000113258444,0.000057456884,0.000034660636,0.00003594665,0.00007978255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024606177,0.00043136333,0.000526074,0.00032248447,0.0007456828,0.0012152137,0.0006127108,0.0007905584,0.0011952189],"category_scores_gemma":[0.001042543,0.0003019808,0.00049084873,0.00027783276,0.0010505414,0.0006994801,0.0006481737,0.00069128786,0.00011100371],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006580015,0.00051527534,0.01653573,0.00011886332,0.00021916814,0.0017602453,0.00054587296,0.9219888,0.039703205,0.012642749,0.0015675517,0.003744549],"study_design_scores_gemma":[0.00022883083,0.00020799151,0.006256863,0.000007910788,0.000021772092,0.00008051577,0.00013173398,0.9871466,0.003183471,0.002341503,0.00036777777,0.000025089703],"about_ca_topic_score_codex":0.0038402264,"about_ca_topic_score_gemma":0.0012269159,"teacher_disagreement_score":0.0038402264,"about_ca_system_score_codex":0.0006565693,"about_ca_system_score_gemma":0.00039615386,"threshold_uncertainty_score":0.007635772},"labels":[],"label_agreement":null},{"id":"W3134320723","doi":"10.3847/1538-4357/abac62","title":"REQUIEM-2D Methodology: Spatially Resolved Stellar Populations of Massive Lensed Quiescent Galaxies from Hubble Space Telescope 2D Grism Spectroscopy","year":2020,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"University of Toronto; Space Telescope Science Institute; National Research Foundation; Alfred P. Sloan Foundation; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Grism; Galaxy; Metallicity; Advanced Camera for Surveys; Hubble space telescope; Stellar mass; Astronomy; Redshift; Star formation; Photometry (optics); Galaxy formation and evolution; Hubble Ultra-Deep Field; Hubble Deep Field; Stars","score_opus":0.03672995094423096,"score_gpt":0.26679960135529757,"score_spread":0.2300696504110666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3134320723","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.10290364,0.00018472115,0.8773498,0.00024668188,0.00004252944,0.00013384032,0.008610734,0.008811003,0.0017170603],"genre_scores_gemma":[0.48167375,0.00012587613,0.49971804,0.00021661015,0.000068146925,0.000350958,0.015056498,0.0011942965,0.0015958045],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99961275,0.0001420404,0.000021050075,0.000111700574,0.00007804526,0.000034446235],"domain_scores_gemma":[0.9985927,0.0005261849,0.00020467464,0.0003894216,0.00018515323,0.00010193451],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021339941,0.0005749626,0.00050257065,0.0011516107,0.00035735435,0.0009217317,0.0018819036,0.00072641246,0.003637217],"category_scores_gemma":[0.0062006395,0.0006712938,0.0009203834,0.0005786844,0.00039127842,0.0008245918,0.0014923264,0.00070223364,0.0008962845],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048702932,0.00024517017,0.16076374,0.0003334572,0.0007466327,0.0003697219,0.000276971,0.6317014,0.0107630165,0.033850826,0.021914855,0.13854721],"study_design_scores_gemma":[0.000041118805,0.000023612409,0.0077053737,0.000015191442,0.00002149061,0.00010615461,0.000019496341,0.97758794,0.0020452335,0.008335163,0.004068513,0.000030692885],"about_ca_topic_score_codex":0.009215664,"about_ca_topic_score_gemma":0.013331538,"teacher_disagreement_score":0.009215664,"about_ca_system_score_codex":0.0006786848,"about_ca_system_score_gemma":0.0010514806,"threshold_uncertainty_score":0.018324018},"labels":[],"label_agreement":null},{"id":"W3134950890","doi":"10.3847/1538-4357/abe6a4","title":"Fitting an Analytic Magnetic Field to a Prestellar Core","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Magnetic field; Polarization (electrochemistry); Radiative transfer; Curvature; Scaling; Magnetic flux; Polarimetry; Magnetic energy; RADIUS","score_opus":0.016323876952893238,"score_gpt":0.2652932942731764,"score_spread":0.24896941732028316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3134950890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96514577,0.000084324354,0.028440086,0.00012793529,0.000017628512,0.000031745425,0.00051420013,0.0004935933,0.0051447707],"genre_scores_gemma":[0.99729115,0.000020605105,0.0021424,0.000015557924,0.0000035836638,0.00001162562,0.00017480098,0.000029659666,0.00031067547],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999442,0.000011645503,0.0000018838186,0.000016279888,0.000012676783,0.0000133373305],"domain_scores_gemma":[0.9998932,0.000028149587,0.000016017277,0.000021870632,0.000028228918,0.0000125613315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015161869,0.00035080744,0.0002168577,0.00029797864,0.00018055076,0.0003680275,0.0005018653,0.00036646886,0.0008491809],"category_scores_gemma":[0.00064348505,0.0001676748,0.00031263876,0.00023863907,0.00020914197,0.00021425333,0.00019381267,0.00018900982,0.00022466472],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000082082006,0.000040370884,0.014187261,0.000030036994,0.000029396419,0.0001491055,0.00008180084,0.96649873,0.01058363,0.0016728392,0.0007121353,0.0059326226],"study_design_scores_gemma":[0.000039100036,0.000031052266,0.0067048436,0.0000038444264,0.000004961265,0.000033414195,0.000031595097,0.98948824,0.0022577415,0.0007504075,0.00064639683,0.0000084440735],"about_ca_topic_score_codex":0.0101317745,"about_ca_topic_score_gemma":0.0040057874,"teacher_disagreement_score":0.0101317745,"about_ca_system_score_codex":0.0005765579,"about_ca_system_score_gemma":0.00044997683,"threshold_uncertainty_score":0.020145595},"labels":[],"label_agreement":null},{"id":"W3135003798","doi":"10.3847/1538-4357/abfa9f","title":"Modeling the Multiwavelength Variability of Mrk 335 Using Gaussian Processes","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science and Technology Facilities Council","keywords":"Gaussian process; Galaxy; Gaussian; Power law; Quadratic equation; Point process; Point spread function; Gaussian function; Spectral density; Quadratic function","score_opus":0.02695746865779842,"score_gpt":0.2599917759143592,"score_spread":0.23303430725656077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135003798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9603039,0.00006987444,0.038046796,0.00015748174,0.000008763253,0.000015967222,0.0001650061,0.000224229,0.0010079903],"genre_scores_gemma":[0.9968454,0.000036558187,0.0025662703,0.000011090623,0.0000035912258,0.000006777086,0.00008438552,0.000018816712,0.00042703084],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987745,0.00003549959,0.0000042743955,0.00003318558,0.000016889253,0.000032602547],"domain_scores_gemma":[0.9992446,0.0003829894,0.00019327365,0.00005957197,0.00006808155,0.000051413444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009432183,0.00038227002,0.00033282218,0.0005318956,0.0002968399,0.0008463213,0.00071149133,0.0007772882,0.0008387691],"category_scores_gemma":[0.00247285,0.00023218818,0.0007361444,0.0004991695,0.00044663754,0.00068967894,0.00035099027,0.0005365021,0.00022722484],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043027554,0.000025967885,0.012913353,0.00000878599,0.000016057871,0.00006350721,0.00004997418,0.9807042,0.0010135849,0.003053416,0.00015257647,0.0019556484],"study_design_scores_gemma":[0.0000049348732,0.000010039117,0.0018495234,0.0000012440823,0.0000040459163,0.000008240511,0.000009356415,0.9974878,0.00012931538,0.00042788166,0.00006293146,0.000004708983],"about_ca_topic_score_codex":0.0421197,"about_ca_topic_score_gemma":0.017151138,"teacher_disagreement_score":0.0421197,"about_ca_system_score_codex":0.0009261231,"about_ca_system_score_gemma":0.0004991295,"threshold_uncertainty_score":0.083749115},"labels":[],"label_agreement":null},{"id":"W3135348024","doi":"10.3847/1538-4357/ac2d2d","title":"Reconstructing the Last Major Merger of the Milky Way with the H3 Survey","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":158,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Milky Way; Halo; Galaxy; Stars; Astronomy; Angular momentum; Galaxy formation and evolution; Population","score_opus":0.01284592671707332,"score_gpt":0.21190102554502718,"score_spread":0.19905509882795386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135348024","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99829084,0.00002892971,0.0005698364,0.00007134379,0.0000040307305,0.0000061965857,0.00024377376,0.000049619342,0.00073534437],"genre_scores_gemma":[0.99897313,0.000010701252,0.00056196115,0.000022676339,0.0000032188368,0.0000039432784,0.00027641616,0.000017875172,0.00013015675],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986935,0.000033713077,0.00000410422,0.000029970653,0.000015990963,0.00004693314],"domain_scores_gemma":[0.9993722,0.00020392807,0.000094785355,0.000087088665,0.00006430598,0.0001776209],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061192934,0.0003300967,0.00039300064,0.00045488923,0.00065729587,0.00077291374,0.0007861456,0.0010648186,0.0016883052],"category_scores_gemma":[0.0017260211,0.00038666045,0.0008926258,0.0005458567,0.00053959276,0.00049967435,0.00078538666,0.00047875088,0.00025650972],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043695804,0.00014289183,0.25700775,0.000035366284,0.00032217082,0.00074670167,0.00033140343,0.73054373,0.0039372738,0.0019966906,0.0010152431,0.0034838025],"study_design_scores_gemma":[0.0002203981,0.00023101157,0.12416204,0.000018942052,0.00009225286,0.00017310336,0.00045316308,0.87017363,0.0015248407,0.0013136064,0.0015912867,0.00004565337],"about_ca_topic_score_codex":0.04706769,"about_ca_topic_score_gemma":0.029603584,"teacher_disagreement_score":0.04706769,"about_ca_system_score_codex":0.0016373799,"about_ca_system_score_gemma":0.0007028087,"threshold_uncertainty_score":0.09358746},"labels":[],"label_agreement":null},{"id":"W3135402511","doi":"10.3847/1538-4357/abeb6c","title":"R Coronae Borealis Star Evolution: Simulating 3D Merger Events to 1D Stellar Evolution Including Large-scale Nucleosynthesis","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Nucleosynthesis; Supergiant; Stellar evolution; Stars; White dwarf; Stellar nucleosynthesis; Abundance (ecology); Red supergiant; Stellar structure; Variable star","score_opus":0.014341823404445116,"score_gpt":0.2490642430348968,"score_spread":0.23472241963045168,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135402511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.992463,0.000047264173,0.002919209,0.00010132803,0.000025567186,0.000032253694,0.00037549232,0.00020631429,0.0038296017],"genre_scores_gemma":[0.9951492,0.000027718514,0.003819971,0.00004372974,0.0000070055044,0.000027067561,0.00029777767,0.000039763934,0.0005877519],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990463,0.000028627368,0.0000053855183,0.000020340887,0.000016427499,0.00002454609],"domain_scores_gemma":[0.99944526,0.00031217726,0.00006167087,0.000034835437,0.000055266813,0.00009074122],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026790853,0.00050886226,0.00041012204,0.00033427542,0.00035367353,0.0006276533,0.000983507,0.0011320334,0.002111399],"category_scores_gemma":[0.0011334211,0.00027507788,0.00069419236,0.00026918846,0.0005053809,0.0003093486,0.00059220457,0.0004924048,0.00015290927],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013999049,0.00012649463,0.0085190255,0.000024350351,0.000040105115,0.00009325297,0.00005264418,0.98709935,0.0016104442,0.0005929504,0.00018687565,0.0015144284],"study_design_scores_gemma":[0.00004442016,0.000046833396,0.0016244123,0.0000022490988,0.000007069403,0.000010094489,0.000028669858,0.9976331,0.00030133378,0.000117886455,0.00017909608,0.0000047292433],"about_ca_topic_score_codex":0.03225691,"about_ca_topic_score_gemma":0.019007675,"teacher_disagreement_score":0.03225691,"about_ca_system_score_codex":0.0008244087,"about_ca_system_score_gemma":0.0006901274,"threshold_uncertainty_score":0.06413829},"labels":[],"label_agreement":null},{"id":"W3135448804","doi":"10.3847/1538-4357/abeb76","title":"Revealing a New Black Widow Binary 4FGL J0336.0+7502","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Research Foundation of Korea","keywords":"Millisecond pulsar; Pulsar; Binary number; Modulation (music); Flux (metallurgy); Telescope; Millisecond; Modulation index","score_opus":0.017888110645389324,"score_gpt":0.24219035242918652,"score_spread":0.2243022417837972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135448804","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978948,0.00020986752,0.00039715183,0.00012475955,0.000029063161,0.000009690562,0.00019539356,0.0000409343,0.001098391],"genre_scores_gemma":[0.9980627,0.000037683927,0.0008905229,0.0001006018,0.000024741028,0.0000047691788,0.0003687428,0.0000061813007,0.00050415966],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987745,0.0000082623255,0.0000058290043,0.000031280095,0.000024193292,0.000052983847],"domain_scores_gemma":[0.9997272,0.000018494624,0.00007310839,0.0000254484,0.000022803144,0.00013304349],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019767258,0.00023544811,0.00032492742,0.00096237945,0.00084827794,0.0007540801,0.0003498007,0.00064029684,0.0023483145],"category_scores_gemma":[0.00035889793,0.00016233268,0.00023116721,0.0005734073,0.00028600427,0.0003201145,0.0007889708,0.00033258714,0.00065761764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014603796,0.0003153762,0.6301189,0.00014727566,0.00009709359,0.017126122,0.0010384753,0.0003623076,0.28909278,0.0024727846,0.0037250617,0.054043427],"study_design_scores_gemma":[0.00014875189,0.0013474803,0.90108067,0.000053881453,0.00011652343,0.028376022,0.001218716,0.0038262992,0.029377503,0.0024158442,0.0319656,0.00007265029],"about_ca_topic_score_codex":0.0014344908,"about_ca_topic_score_gemma":0.0016773391,"teacher_disagreement_score":0.0023483145,"about_ca_system_score_codex":0.00029679068,"about_ca_system_score_gemma":0.00015163778,"threshold_uncertainty_score":0.007855833},"labels":[],"label_agreement":null},{"id":"W3135464666","doi":"10.3847/1538-4357/ac0f5b","title":"Probing Intra-Halo Light with Galaxy Stacking in CIBER Images","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Carnegie Institution of Washington; Planetary Science Division; Queen's University; Japan Society for the Promotion of Science; Integrated Electronics Engineering Center, Binghamton University; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; European Space Agency; Smithsonian Astrophysical Observatory; Office of Science; University of Colorado Boulder; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; NASA Headquarters; Max-Planck-Institut für Astronomie; Space Telescope Science Institute; Institut de Física d'Altes Energies; Eötvös Loránd Tudományegyetem; Ministry of Education, Culture, Sports, Science and Technology; National Central University; Max-Planck-Institut für Astrophysik; Nuclear Safety and Security Commission; York University; Ministério da Ciência, Tecnologia e Inovação; Gordon and Betty Moore Foundation; Queen's University Belfast; University of Oxford; Durham University; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Science Mission Directorate; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; University of Portsmouth; New Mexico State University; University of Utah; Ohio State University; Smithsonian Institution; Yale University; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Vanderbilt University; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Halo; Astronomy; Surface brightness fluctuation; Surface brightness; Sky; Luminous infrared galaxy; Brightest cluster galaxy","score_opus":0.0056520928511841605,"score_gpt":0.2015798027814985,"score_spread":0.19592770993031436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3135464666","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99769163,0.000034991182,0.0016153649,0.000007654173,0.000001341624,0.000003898491,0.00020582785,0.00008868735,0.0003506703],"genre_scores_gemma":[0.9972594,0.000015091452,0.0020244336,0.000008069848,0.0000043775494,0.0000021670585,0.00059684523,0.000014394035,0.00007529416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996911,0.000041000167,0.000009868016,0.000083970655,0.00009130057,0.00008275203],"domain_scores_gemma":[0.9991721,0.00011380276,0.00027437284,0.00014907437,0.00013215988,0.0001584765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007984833,0.00042831828,0.00030291622,0.0018755391,0.0002465963,0.0005121458,0.0003276649,0.00020722549,0.0004925571],"category_scores_gemma":[0.0010288673,0.00020390624,0.0003539103,0.00088359124,0.00027148027,0.00031455487,0.00045833888,0.00019331949,0.00017533232],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000241042,0.00007481974,0.92473453,0.000028104321,0.00022182059,0.00011365144,0.00030329492,0.011544726,0.043805115,0.0004761775,0.0003808815,0.01807588],"study_design_scores_gemma":[0.0000036344318,0.00003623843,0.9675184,0.0000036884844,0.000032632615,0.000058987393,0.00007327726,0.025339844,0.0064272517,0.00016376998,0.00033134513,0.000010979934],"about_ca_topic_score_codex":0.0049177175,"about_ca_topic_score_gemma":0.0081351865,"teacher_disagreement_score":0.0049177175,"about_ca_system_score_codex":0.0003674093,"about_ca_system_score_gemma":0.00012454916,"threshold_uncertainty_score":0.009778202},"labels":[],"label_agreement":null},{"id":"W3136467459","doi":"10.3847/1538-4357/abf1e7","title":"The Fundamental Plane in the LEGA-C Survey: Unraveling the M/L Ratio Variations of Massive Star-forming and Quiescent Galaxies at z ∼ 0.8","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Galaxy; Astrophysics","score_opus":0.011951466914743015,"score_gpt":0.22314461298612673,"score_spread":0.2111931460713837,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3136467459","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947455,0.00017579769,0.00027634713,0.000092434224,0.0000029330185,0.000003300302,0.0032730657,0.000034004162,0.0013965552],"genre_scores_gemma":[0.9946884,0.000067969835,0.0003740008,0.000036080404,0.000008939516,0.000004767123,0.0045501227,0.000012760598,0.00025712777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998317,0.00003061041,0.0000066426373,0.000051646573,0.000029524283,0.000049784307],"domain_scores_gemma":[0.9990127,0.0001498323,0.000429112,0.000097296,0.00010584239,0.0002051544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037098257,0.00017039785,0.00019732288,0.0020626916,0.00023916432,0.00097247673,0.00025398587,0.00023724702,0.0010781618],"category_scores_gemma":[0.0012052251,0.00013140692,0.00020633452,0.0015358976,0.00024256148,0.00042762616,0.00066340895,0.00021975109,0.00046476827],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006293904,0.0000098306,0.9897634,0.00000891999,0.000024463523,0.000032631546,0.00017494409,0.00014340367,0.0026762297,0.0002794812,0.0008173314,0.0060063386],"study_design_scores_gemma":[0.000001651183,0.000004603241,0.99890363,0.0000022118165,0.000002906344,0.000019565123,0.000040547926,0.0003038746,0.000081532395,0.00005122869,0.00058652373,0.0000016316334],"about_ca_topic_score_codex":0.021275312,"about_ca_topic_score_gemma":0.02545498,"teacher_disagreement_score":0.021275312,"about_ca_system_score_codex":0.0004137018,"about_ca_system_score_gemma":0.0001880126,"threshold_uncertainty_score":0.042302966},"labels":[],"label_agreement":null},{"id":"W3136528259","doi":"10.3847/1538-4357/abee13","title":"The Role of Adaptive Ray Tracing in Analyzing Black Hole Structure","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Gordon and Betty Moore Foundation","keywords":"Supermassive black hole; Ray tracing (physics); Black hole (networking); Radiative transfer; Computation; Interferometry; X-ray telescope; Event horizon","score_opus":0.008242373206980964,"score_gpt":0.22022285342671796,"score_spread":0.211980480219737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3136528259","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7482302,0.0001406751,0.246709,0.0002838404,0.000027070633,0.00004726572,0.000080402235,0.0009514148,0.0035301426],"genre_scores_gemma":[0.93861073,0.000035361176,0.06095419,0.000023552902,0.0000066852335,0.000009894033,0.000030864958,0.00008966694,0.00023906758],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990535,0.00004245165,0.0000036732201,0.000011694853,0.00002413122,0.000012728866],"domain_scores_gemma":[0.99929225,0.0003954663,0.00008344303,0.00010306099,0.00006518971,0.00006059556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060669816,0.00035466638,0.00024517794,0.0005063072,0.0002892306,0.00067252683,0.00067653495,0.0004016753,0.00080947665],"category_scores_gemma":[0.0029072503,0.00020653981,0.0001835779,0.00033808273,0.0006021524,0.0005553878,0.0006064019,0.0004332712,0.000091661925],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012783121,0.000057408957,0.007406853,0.000022275042,0.000035174813,0.00008680804,0.000097847034,0.95717806,0.013962031,0.006735538,0.00019691589,0.01409332],"study_design_scores_gemma":[0.0000058106907,0.000005524195,0.0003049965,9.672374e-7,9.976735e-7,0.000005222975,0.000005233985,0.99800295,0.0008861107,0.0007257499,0.000054298358,0.0000020798097],"about_ca_topic_score_codex":0.004834225,"about_ca_topic_score_gemma":0.0032075713,"teacher_disagreement_score":0.004834225,"about_ca_system_score_codex":0.0005248164,"about_ca_system_score_gemma":0.00044789785,"threshold_uncertainty_score":0.009612203},"labels":[],"label_agreement":null},{"id":"W3136589136","doi":"10.3847/1538-4357/abee91","title":"New Experimental <sup>23</sup>Na(α, p)<sup>26</sup>Mg Reaction Rate for Massive Star and Type Ia Supernova Models","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"Magyar Tudományos Akadémia; European Cooperation in Science and Technology; University of Hull; Central Laser Facility, Science and Technology Facilities Council; Science and Technology Facilities Council; European Research Council; National Science Foundation","keywords":"Physics; Supernova; Astrophysics; Nucleosynthesis; Star (game theory); Nuclear reaction; Stellar evolution; Nuclear physics; Astronomy; Stars","score_opus":0.02707883057437331,"score_gpt":0.2982916300212534,"score_spread":0.2712127994468801,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3136589136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8877083,0.0013845864,0.08767793,0.0001365626,0.00013563766,0.0001273525,0.0054617664,0.0012709983,0.016096808],"genre_scores_gemma":[0.9886314,0.00025621825,0.0071189767,0.000024416584,0.0000310021,0.00007688652,0.0027572736,0.00019686871,0.0009069288],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9991423,0.00019336447,0.000064175896,0.00025975204,0.0002628824,0.000077477824],"domain_scores_gemma":[0.9970119,0.001283191,0.00071529875,0.00065265043,0.0002472077,0.00008971758],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025717167,0.0012828106,0.0005658735,0.00095541414,0.00028902252,0.0010397305,0.001622556,0.000609931,0.0033595979],"category_scores_gemma":[0.0031746952,0.00041669345,0.001416883,0.00049641693,0.00046881064,0.0008614459,0.0007162191,0.0004814289,0.0009133636],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0050354865,0.0006591875,0.21746124,0.0012405041,0.0010764496,0.0016887095,0.00024644006,0.5238071,0.16296996,0.026642207,0.0031287195,0.056044057],"study_design_scores_gemma":[0.00025035703,0.0005195231,0.07246753,0.00007133705,0.0006157646,0.00079967076,0.000074581985,0.69019055,0.21552734,0.008736053,0.010520294,0.00022697475],"about_ca_topic_score_codex":0.001705061,"about_ca_topic_score_gemma":0.0017282746,"teacher_disagreement_score":0.0033595979,"about_ca_system_score_codex":0.0008003604,"about_ca_system_score_gemma":0.00027752697,"threshold_uncertainty_score":0.013600707},"labels":[],"label_agreement":null},{"id":"W3136892902","doi":"10.3847/1538-4357/ac20df","title":"A Constraint on Primordial B-modes from the First Flight of the Spider Balloon-borne Telescope","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"Fermilab; British Antarctic Survey; British Columbia Knowledge Development Fund; Office of Science; Norges Forskningsråd; Science and Technology Facilities Council; University of Toronto; Canadian Space Agency; Inyuvesi Yakwazulu-Natali; UK Research and Innovation; National Science Foundation; Compute Canada; David and Lucile Packard Foundation; University of Texas at Austin; U.S. Department of Energy; Princeton University; Science Mission Directorate; Government of Ontario; National Aeronautics and Space Administration; Vetenskapsrådet","keywords":"Physics; Cosmic microwave background; Planck; Astrophysics; Spectral density; Cosmic background radiation; Polarization (electrochemistry); Astronomy; Anisotropy; Optics","score_opus":0.007310538605871642,"score_gpt":0.22240064690340053,"score_spread":0.2150901082975289,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3136892902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.937433,0.00035765243,0.05012011,0.00036471518,0.000036574602,0.000013377507,0.0014358878,0.00047302688,0.009765708],"genre_scores_gemma":[0.99183077,0.000047108962,0.006827754,0.000072860596,0.000019862242,0.000007232934,0.00093363365,0.000059124966,0.00020171497],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990299,0.0002049694,0.000052128882,0.00029762325,0.0002909296,0.00012443848],"domain_scores_gemma":[0.9947935,0.0022062175,0.0008246473,0.0012337113,0.00044572487,0.00049617904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023012124,0.00047941695,0.0004395445,0.00064895407,0.0005533184,0.0011970385,0.0005612254,0.00046379885,0.0018356451],"category_scores_gemma":[0.007420413,0.00045076717,0.0006171054,0.0003810973,0.00048111126,0.00059305044,0.00092104427,0.0005945768,0.0004863126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056124595,0.00008440004,0.7628328,0.00016740941,0.0003224606,0.00037092908,0.00062935683,0.019444712,0.1413909,0.031973016,0.0029931972,0.039229553],"study_design_scores_gemma":[0.000106271764,0.0001771844,0.7921133,0.00011370111,0.0001789848,0.0007657633,0.00022167111,0.11926722,0.052624114,0.021357717,0.012928475,0.00014555137],"about_ca_topic_score_codex":0.0039345794,"about_ca_topic_score_gemma":0.0039804867,"teacher_disagreement_score":0.0039345794,"about_ca_system_score_codex":0.00045407235,"about_ca_system_score_gemma":0.00061979407,"threshold_uncertainty_score":0.012170136},"labels":[],"label_agreement":null},{"id":"W3136957856","doi":"10.3847/1538-4357/ac33ac","title":"Fast Radio Burst Morphology in the First CHIME/FRB Catalog","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; University of Waterloo; National Research Council Canada; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; McGill Space Institute; National Research Council Canada; University of Toronto; Industry Canada; Canada Research Chairs; National Science Foundation; Government of Canada; Smithsonian Astrophysical Observatory; U.S. Department of Defense; McGill University; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Canadian Institute for Advanced Research","keywords":"Fast radio burst; Computer science; Astronomy; Physics","score_opus":0.011290681895811625,"score_gpt":0.2931440426125453,"score_spread":0.28185336071673367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3136957856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.924193,0.0010358226,0.0018349356,0.00015294725,0.000026858992,0.00018064331,0.055708013,0.00071044813,0.016157316],"genre_scores_gemma":[0.8867771,0.0007636666,0.0059388517,0.00009595242,0.000036188227,0.00014831667,0.100955136,0.00033417638,0.0049506743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992562,0.000029521785,0.000043792992,0.00016964007,0.0003406137,0.00016022263],"domain_scores_gemma":[0.9958103,0.0003981577,0.0008300052,0.0007639784,0.0017490191,0.0004485727],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009918663,0.0004188232,0.00045950428,0.00866329,0.0008007006,0.0014605778,0.00059310696,0.00025749725,0.004131509],"category_scores_gemma":[0.0045399917,0.00023077414,0.00027883105,0.0068172626,0.00035395482,0.00053947244,0.0011893604,0.00025735388,0.0012958341],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025761916,0.00003689705,0.8948666,0.0001664033,0.000109912056,0.00033573387,0.0011382583,0.0007529845,0.014097814,0.00085638545,0.01341933,0.07396216],"study_design_scores_gemma":[0.000004082599,0.0000072205003,0.9903854,0.000015785663,0.0000135950695,0.00010515354,0.00015761603,0.00020971014,0.0005645734,0.00006364329,0.008462904,0.000010241467],"about_ca_topic_score_codex":0.22597949,"about_ca_topic_score_gemma":0.3313029,"teacher_disagreement_score":0.7740205,"about_ca_system_score_codex":0.0021013222,"about_ca_system_score_gemma":0.0016435926,"threshold_uncertainty_score":0.4493283},"labels":[],"label_agreement":null},{"id":"W3137205034","doi":"10.3847/1538-4357/abec81","title":"Cosmic Evolution of the H<sub>2</sub> Mass Density and the Epoch of Molecular Gas","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Star formation; Galaxy; Redshift; Epoch (astronomy); COSMIC cancer database; Interstellar medium; Galaxy formation and evolution; Stellar mass; Sky; Infrared","score_opus":0.0033963900363618072,"score_gpt":0.1784039687286055,"score_spread":0.1750075786922437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3137205034","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964259,0.00012858113,0.00041168628,0.00006740045,0.0000028882757,0.0000015197111,0.0009887625,0.000021985914,0.0019512883],"genre_scores_gemma":[0.9991829,0.000036244914,0.00011443194,0.000011068401,0.0000065542336,0.0000012532379,0.0004439683,0.000004837428,0.00019876807],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988973,0.000021700025,0.000007314549,0.000032393626,0.00002709724,0.000021824137],"domain_scores_gemma":[0.99762124,0.0005762604,0.0010924572,0.0002805376,0.00015638932,0.00027307135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033307867,0.00013131823,0.000114186834,0.00084566843,0.00015247088,0.00070475414,0.00019547032,0.0001944746,0.002313981],"category_scores_gemma":[0.0020391673,0.00013243528,0.00014635842,0.0006129298,0.00037516258,0.00036370743,0.0003475843,0.00023063115,0.00038384504],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005986326,0.000010764854,0.989881,0.000010689876,0.000040997053,0.000052266925,0.000097243494,0.00080978003,0.0033602468,0.0014827658,0.00034669618,0.0038476805],"study_design_scores_gemma":[7.850459e-7,0.000005728926,0.9985031,0.0000019126721,0.000003787958,0.000028614571,0.000015232401,0.0006770454,0.00030749573,0.00014407554,0.0003102472,0.000002035526],"about_ca_topic_score_codex":0.006467055,"about_ca_topic_score_gemma":0.009078356,"teacher_disagreement_score":0.006467055,"about_ca_system_score_codex":0.00048347423,"about_ca_system_score_gemma":0.00009541309,"threshold_uncertainty_score":0.012858808},"labels":[],"label_agreement":null},{"id":"W3137366937","doi":"10.3847/1538-4357/abed4c","title":"The Be Star 66 Ophiuchi: 60 Years of Disk Evolution","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Position angle; Dissipation; Polarization (electrochemistry); RADIUS; Monte Carlo method; Thick disk; Debris disk; Thin disk","score_opus":0.009634536755215662,"score_gpt":0.22074818031085874,"score_spread":0.21111364355564308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3137366937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985096,0.000045934736,0.00035033817,0.000028569712,0.0000017921956,0.0000043173936,0.0005498405,0.000026300884,0.00048328546],"genre_scores_gemma":[0.9981389,0.00004584457,0.00037141202,0.000007902387,0.000002477932,0.0000050986473,0.0012211578,0.000011956066,0.00019519919],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998913,0.000016932467,0.000008622835,0.000032478925,0.000026846132,0.000023867882],"domain_scores_gemma":[0.9997365,0.000081486134,0.000058707934,0.000035081528,0.00003830216,0.00004990467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034081642,0.00025100412,0.00033575593,0.00048573583,0.000598369,0.0005757548,0.0002804371,0.00034421516,0.0006888286],"category_scores_gemma":[0.0012864769,0.00021655025,0.00031701155,0.00062917033,0.00030869045,0.00051313266,0.0005906831,0.0002977401,0.00017561961],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030874688,0.00014922579,0.81594354,0.0000963373,0.00019939919,0.001256292,0.00077800895,0.15918773,0.0082514,0.0012189778,0.00079825416,0.011812001],"study_design_scores_gemma":[0.000052531606,0.0002222741,0.6768862,0.000028624281,0.00008789246,0.0005566747,0.00041127478,0.31012005,0.0052552205,0.0012374726,0.0050814776,0.000060309347],"about_ca_topic_score_codex":0.02921907,"about_ca_topic_score_gemma":0.022091491,"teacher_disagreement_score":0.02921907,"about_ca_system_score_codex":0.0008682461,"about_ca_system_score_gemma":0.00035571304,"threshold_uncertainty_score":0.05809796},"labels":[],"label_agreement":null},{"id":"W3137594256","doi":"10.3847/1538-4357/abed4d","title":"The HST See Change Program. I. Survey Design, Pipeline, and Supernova Discoveries*","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; York University","funders":"Science and Technology Facilities Council","keywords":"Redshift; Physics; Supernova; Astrophysics; Photometry (optics); Galaxy; Cosmology; Astronomy; Hubble space telescope; Galaxy cluster; Cluster (spacecraft); Dark energy; Weak gravitational lensing; Stars; Computer science","score_opus":0.03595586904286305,"score_gpt":0.26523083493808536,"score_spread":0.2292749658952223,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3137594256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.40077066,0.0002955218,0.1892143,0.0014450387,0.0002033076,0.015891174,0.23688816,0.10895409,0.046337757],"genre_scores_gemma":[0.44993544,0.00019911786,0.27705643,0.00094600004,0.00025291578,0.011170229,0.24132028,0.0037312908,0.015388379],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987921,0.0002958078,0.000052796975,0.00027678258,0.00043433896,0.00014823712],"domain_scores_gemma":[0.9979955,0.00031757628,0.00028241135,0.00044886945,0.00063272496,0.0003229868],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002153907,0.00049497915,0.00033084024,0.0020592385,0.0004507831,0.00065507327,0.0007911952,0.0002808837,0.008801599],"category_scores_gemma":[0.0032431353,0.00051771395,0.00031426892,0.0016686678,0.00028558436,0.00054574927,0.000993483,0.0002922024,0.0072995326],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0030874186,0.0008207008,0.3694505,0.00033526673,0.00013408232,0.00032364836,0.0005347353,0.010132311,0.049625475,0.0027257367,0.20756033,0.3552698],"study_design_scores_gemma":[0.0011461419,0.00252082,0.6163586,0.000055333014,0.00012026811,0.0006821458,0.00046224988,0.14273359,0.048482604,0.002786873,0.18450649,0.00014494685],"about_ca_topic_score_codex":0.009595956,"about_ca_topic_score_gemma":0.014247076,"teacher_disagreement_score":0.009595956,"about_ca_system_score_codex":0.0007174757,"about_ca_system_score_gemma":0.0010294719,"threshold_uncertainty_score":0.029444337},"labels":[],"label_agreement":null},{"id":"W3137722370","doi":"10.3847/1538-4357/ac05cc","title":"Modeling the Sgr A* Black Hole Immersed in a Dark Matter Spike","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":106,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Quantum Research Center","funders":"Natural Science Foundation of Zhejiang Province; National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Milky Way; Dark matter; Galaxy; Black hole (networking); RADIUS; Dark matter halo; Accretion (finance); Spike (software development); Halo; Astronomy","score_opus":0.016044413850079934,"score_gpt":0.23645148219862436,"score_spread":0.22040706834854443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3137722370","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9800576,0.00009221084,0.01463275,0.00027525972,0.000028182294,0.000024145213,0.00013197173,0.00007900724,0.004678842],"genre_scores_gemma":[0.9972874,0.00003680516,0.0017831478,0.000036573107,0.000014429569,0.000009148371,0.00006055074,0.000019382547,0.00075266947],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992883,0.000020648848,0.000002987679,0.000013673068,0.000011125023,0.000022727341],"domain_scores_gemma":[0.99957365,0.00011033754,0.00007993728,0.000035383262,0.000040150702,0.00016051337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027093187,0.0004921014,0.00051872927,0.00033708778,0.00060510804,0.0010155293,0.0010415383,0.0014661994,0.0018473371],"category_scores_gemma":[0.0010433313,0.00030643263,0.00060923846,0.00020580912,0.001102628,0.000820525,0.0015237108,0.00059420266,0.00019472753],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027350461,0.00008020121,0.01412236,0.0000456619,0.0000792592,0.0014524509,0.00012771084,0.9568303,0.0085624475,0.016340284,0.0004668524,0.0016190177],"study_design_scores_gemma":[0.000048104255,0.00006843516,0.0027943468,0.0000043945843,0.000015570185,0.00008241106,0.000067363195,0.99349976,0.0005022768,0.0026642457,0.0002387128,0.0000144538635],"about_ca_topic_score_codex":0.010924991,"about_ca_topic_score_gemma":0.0037799464,"teacher_disagreement_score":0.010924991,"about_ca_system_score_codex":0.000846567,"about_ca_system_score_gemma":0.00051756296,"threshold_uncertainty_score":0.021722794},"labels":[],"label_agreement":null},{"id":"W3138127556","doi":"10.3847/1538-4357/abef6b","title":"Puffed-up Edges of Planet-opened Gaps in Protoplanetary Disks. I. Hydrodynamic Simulations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Planet; Protoplanetary disk; Millimeter; Dust lane; Scale height; Trapping; Zonal and meridional","score_opus":0.009713147689810827,"score_gpt":0.2406046904864658,"score_spread":0.23089154279665497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3138127556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97902495,0.00028223204,0.0031522892,0.000728715,0.00007994531,0.00009504874,0.0022226786,0.00032293142,0.0140911685],"genre_scores_gemma":[0.99474853,0.00011694816,0.0025750503,0.00020169365,0.000030901087,0.00007144433,0.00093302364,0.00008217282,0.0012401142],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998294,0.000039429062,0.000008186805,0.000027917238,0.000028047656,0.00006693524],"domain_scores_gemma":[0.99882835,0.0005197643,0.00015051106,0.00008830555,0.0001202826,0.00029275805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000417993,0.0006419564,0.0009272573,0.0006639542,0.0009483981,0.001105634,0.0017282795,0.0022095838,0.003856521],"category_scores_gemma":[0.0022174118,0.00054240826,0.0009923157,0.0005288107,0.0014266091,0.0007469645,0.0012078494,0.001457054,0.00034565732],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027470387,0.00028985253,0.013843482,0.00008020034,0.00008513403,0.00028146297,0.00014815545,0.9773801,0.0011214478,0.0036703935,0.001319293,0.0015058216],"study_design_scores_gemma":[0.00016702045,0.000059433998,0.002695265,0.000015051808,0.000015295142,0.000019951782,0.0000793467,0.99521184,0.00021506085,0.0011338468,0.00037424473,0.000013656593],"about_ca_topic_score_codex":0.047130175,"about_ca_topic_score_gemma":0.020513253,"teacher_disagreement_score":0.047130175,"about_ca_system_score_codex":0.0017394528,"about_ca_system_score_gemma":0.0011290261,"threshold_uncertainty_score":0.093711674},"labels":[],"label_agreement":null},{"id":"W3138685979","doi":"10.3847/1538-4357/abdd1e","title":"A Multi–Observing Technique Study of the Dynamical Evolution of the Viscous Disk around the Be Star ω CMa","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Balmer series; Astrophysics; Radiative transfer; Be star; Photometry (optics); Stars; Dissipation; Thin disk; Light curve; Thick disk; Spectral line; Debris disk; Emission spectrum; Computational physics; Astronomy; Optics; Planetary system; Thermodynamics","score_opus":0.012615371664155502,"score_gpt":0.2505729808010327,"score_spread":0.2379576091368772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3138685979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983657,0.00002125148,0.0012000288,0.000006864077,9.802726e-7,0.0000025818642,0.0000659527,0.000027787453,0.00030899368],"genre_scores_gemma":[0.998601,0.000011565995,0.0011293712,0.0000022596955,0.0000014440592,0.0000023690127,0.00012834718,0.000005932308,0.00011767504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999294,0.000011059349,0.0000025425152,0.000030683554,0.000013633688,0.000012741293],"domain_scores_gemma":[0.99975103,0.00005786991,0.00006327529,0.00004068346,0.000034865177,0.000052190444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019547778,0.00017496273,0.00017896328,0.00050255796,0.00030434944,0.00022677834,0.0002018548,0.00021135187,0.0004720762],"category_scores_gemma":[0.00035132654,0.00014426936,0.0002995515,0.00029161017,0.00012381772,0.0002699989,0.00031228366,0.00021603964,0.00012964456],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047912786,0.00041429725,0.5519967,0.00006681351,0.00021207193,0.00049152,0.00042921436,0.057565592,0.35916695,0.00093081506,0.00028539667,0.027961554],"study_design_scores_gemma":[0.000012799809,0.00026409468,0.8197354,0.000005701252,0.000046701447,0.000224812,0.000107413485,0.15952548,0.01908703,0.00021920231,0.0007504697,0.000020970385],"about_ca_topic_score_codex":0.0018610655,"about_ca_topic_score_gemma":0.0019986322,"teacher_disagreement_score":0.0018610655,"about_ca_system_score_codex":0.00022215249,"about_ca_system_score_gemma":0.00009008535,"threshold_uncertainty_score":0.0037004352},"labels":[],"label_agreement":null},{"id":"W3138705197","doi":"10.3847/1538-4357/abf35b","title":"The Organization of Cloud-scale Gas Density Structure: High-resolution CO versus 3.6 μm Brightness Contrasts in Nearby Galaxies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Ministerio de Ciencia e Innovación; National Science Council; Deutsche Forschungsgemeinschaft; National Astronomical Observatory of Japan; European Commission; National Institutes of Natural Sciences; Ministerio de Ciencia, Innovación y Universidades; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Agencia Estatal de Investigación; National Radio Astronomy Observatory; National Science Foundation","keywords":"Galaxy; Spiral galaxy; Surface brightness; Bar (unit); Interstellar medium; Spiral (railway); Brightness; Stellar mass; Mass distribution","score_opus":0.0047035693440053705,"score_gpt":0.20025919611211165,"score_spread":0.19555562676810628,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3138705197","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99937004,0.000033527507,0.00015754324,0.0000073270517,4.722904e-7,9.054447e-7,0.00007127382,0.00001045438,0.0003484724],"genre_scores_gemma":[0.99983394,0.0000049011855,0.00007615065,0.0000030314898,0.0000011493877,5.4567414e-7,0.0000595742,0.0000018753874,0.00001868836],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988854,0.000012596277,0.0000055380215,0.0000344821,0.000028005185,0.000030890904],"domain_scores_gemma":[0.9993298,0.0001327691,0.00025016893,0.000059487633,0.000094261755,0.00013360997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016813829,0.00009132376,0.00016942853,0.0011462518,0.00023890453,0.00061368884,0.00019776948,0.00020923471,0.0006062135],"category_scores_gemma":[0.000834502,0.000121579564,0.00014479955,0.00055476616,0.0003421724,0.0002954567,0.0004074822,0.0001540537,0.0001673528],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000948958,0.000013653186,0.97072303,0.000008757025,0.000027779335,0.0000693751,0.00021874138,0.00041325556,0.025060186,0.00015362266,0.00006488164,0.0031519101],"study_design_scores_gemma":[5.30467e-7,0.000005920358,0.999116,7.9910353e-7,0.0000020469872,0.000033437092,0.000053091695,0.0003168124,0.00040530157,0.000028750777,0.000035795732,0.0000014196899],"about_ca_topic_score_codex":0.0039071073,"about_ca_topic_score_gemma":0.0053379796,"teacher_disagreement_score":0.0039071073,"about_ca_system_score_codex":0.00025592395,"about_ca_system_score_gemma":0.000082119004,"threshold_uncertainty_score":0.00776875},"labels":[],"label_agreement":null},{"id":"W3139024047","doi":"10.3847/1538-4357/abfa13","title":"Expanded Atmospheres and Winds in Type I X-Ray Bursts from Accreting Neutron Stars","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; McGill University Health Centre","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China","keywords":"Physics; Neutron star; Astrophysics; Astronomy; Stars; Stellar wind","score_opus":0.013182527813460408,"score_gpt":0.23709835969539006,"score_spread":0.22391583188192965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3139024047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969223,0.000028375936,0.0018263796,0.000027320953,0.0000050286662,0.0000039790725,0.00007916052,0.000031370622,0.0010761595],"genre_scores_gemma":[0.9990355,0.000026953985,0.00047170318,0.0000065477134,0.0000030459223,0.000005879321,0.0001114227,0.00001395321,0.00032503429],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999174,0.000023414794,0.000007273557,0.0000149091475,0.000016550614,0.000020402967],"domain_scores_gemma":[0.9996259,0.00015287762,0.000084545485,0.00003106131,0.000044645185,0.000060930677],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032456795,0.00043567503,0.00032046842,0.00042536968,0.00043569287,0.0006957776,0.0006078311,0.00066367455,0.0014101852],"category_scores_gemma":[0.001488736,0.00036825633,0.00076251844,0.0003088332,0.0003943126,0.00045258863,0.0004692683,0.00040791457,0.00012817809],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007845372,0.00003795326,0.039553348,0.000020541487,0.00005283529,0.00031134541,0.000082837956,0.9538067,0.0024646332,0.0020155923,0.00010539276,0.0014703075],"study_design_scores_gemma":[0.00002855057,0.000064081534,0.018775325,0.00000829243,0.000019533552,0.00008046054,0.00006953159,0.978675,0.0010632465,0.0010199072,0.0001830801,0.000012889273],"about_ca_topic_score_codex":0.00799191,"about_ca_topic_score_gemma":0.0033047793,"teacher_disagreement_score":0.00799191,"about_ca_system_score_codex":0.0006296155,"about_ca_system_score_gemma":0.00028174007,"threshold_uncertainty_score":0.015890777},"labels":[],"label_agreement":null},{"id":"W3139110896","doi":"10.3847/1538-4357/abefd4","title":"Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves. I. Period–Fourier–Metallicity Relations for Fundamental-mode RR Lyrae","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"RR Lyrae variable; Metallicity; Globular cluster; Stars; Infrared; Spitzer Space Telescope; Spectroscopy; Calibration; Variable star","score_opus":0.014741315316075351,"score_gpt":0.2599492644832038,"score_spread":0.24520794916712846,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3139110896","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897271,0.00089430617,0.0024528129,0.000047444115,0.000011683812,0.0000120566165,0.0013918998,0.00020017147,0.005262479],"genre_scores_gemma":[0.9970656,0.00012919707,0.0010444418,0.000015260164,0.000013397335,0.000005614061,0.001467392,0.000030632076,0.00022849363],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997801,0.000021294258,0.000017928449,0.000086204825,0.00006209095,0.000032410033],"domain_scores_gemma":[0.9993611,0.00007702375,0.00028355312,0.00011217839,0.00010451819,0.000061674145],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041875575,0.00036669913,0.00019613326,0.00274325,0.00020295173,0.00055507926,0.00028428205,0.00033614252,0.0007465709],"category_scores_gemma":[0.0009777206,0.00016251064,0.00029355107,0.0010534618,0.00024001273,0.0004264192,0.00045775904,0.00025852106,0.0008538133],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000088004635,0.00002817947,0.9486125,0.00005463212,0.000066677305,0.00006824373,0.00018619641,0.0026152614,0.020501677,0.0005032045,0.0008590266,0.026416335],"study_design_scores_gemma":[0.0000032638904,0.00001640659,0.99337935,0.000008767705,0.000011956521,0.00007293449,0.000045855802,0.0028221402,0.0019761866,0.00016691002,0.0014897371,0.000006559023],"about_ca_topic_score_codex":0.0025677348,"about_ca_topic_score_gemma":0.0028427974,"teacher_disagreement_score":0.00274325,"about_ca_system_score_codex":0.0004036864,"about_ca_system_score_gemma":0.00011007394,"threshold_uncertainty_score":0.005105555},"labels":[],"label_agreement":null},{"id":"W3139497380","doi":"10.3847/1538-4357/abec6e","title":"Discovery of an Edge-on Circumstellar Debris Disk around BD+45° 598: A Newly Identified Member of the β Pictoris Moving Group","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Université de Montréal; Rio Tinto (Canada); Herzberg Institute of Astrophysics; Espace pour la vie","funders":"Science and Technology Facilities Council","keywords":"Debris disk; Plateau de Bure Interferometer; Debris; Circumstellar dust; Population; Thick disk; Luminosity; Planetary system; Circumstellar disk","score_opus":0.012379534675396618,"score_gpt":0.2398841812824828,"score_spread":0.22750464660708616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3139497380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986727,0.000060946233,0.00013825663,0.00001624795,0.0000064184987,0.000004289733,0.00005558248,0.000006072527,0.0010395674],"genre_scores_gemma":[0.99939704,0.000029967014,0.00023617728,0.00002681966,0.000009487132,0.0000022551476,0.00011728689,0.0000024839035,0.00017848505],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991274,0.000004177693,0.0000064341834,0.000028974555,0.000021934977,0.000025711783],"domain_scores_gemma":[0.99978036,0.00001215576,0.00006253708,0.000018158205,0.000026407592,0.00010028971],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109917535,0.00023049771,0.00023941143,0.0006519305,0.0007803507,0.00064743153,0.000287946,0.00032431155,0.0012729167],"category_scores_gemma":[0.00019893241,0.00015425037,0.00014208621,0.00033903663,0.00025053622,0.00021744262,0.00046957727,0.00027711212,0.000545444],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027309396,0.000101664366,0.8400436,0.00004229187,0.00003383601,0.0043168245,0.00077518285,0.000059953723,0.14415286,0.00019828959,0.00029664687,0.009705768],"study_design_scores_gemma":[0.000008290877,0.00018946025,0.98736876,0.000010544734,0.000021669926,0.004864399,0.00045153408,0.00017881884,0.004157334,0.00007418932,0.0026695768,0.000005435382],"about_ca_topic_score_codex":0.0012327255,"about_ca_topic_score_gemma":0.0019575357,"teacher_disagreement_score":0.0012729167,"about_ca_system_score_codex":0.00017798494,"about_ca_system_score_gemma":0.00008360448,"threshold_uncertainty_score":0.0042583346},"labels":[],"label_agreement":null},{"id":"W3139931002","doi":"10.3847/1538-4357/abf3ca","title":"The JCMT BISTRO-2 Survey: The Magnetic Field in the Center of the Rosette Molecular Cloud","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"National Key Research and Development Program of China; Science and Technology Facilities Council; Ministry of Science and Technology, Taiwan; National Natural Science Foundation of China; National Foundation for Science and Technology Development","keywords":"Magnetic field; James Clerk Maxwell Telescope; Polarization (electrochemistry); Molecular cloud; Rosette (schizont appearance); Infrared; Planck; Protein filament","score_opus":0.007574475879718228,"score_gpt":0.2283842683112481,"score_spread":0.22080979243152987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3139931002","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99728584,0.00006688867,0.00012585393,0.000033094515,0.0000036435695,0.0000060524176,0.0011936441,0.000026400401,0.0012585795],"genre_scores_gemma":[0.99639976,0.000041473417,0.00056526426,0.000033615834,0.000013657843,0.0000069231737,0.0026088245,0.000012927138,0.00031761476],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998336,0.000018889792,0.000007788652,0.000047779624,0.000045669836,0.000046349625],"domain_scores_gemma":[0.99952626,0.00003093518,0.00014605788,0.000073073905,0.00008514217,0.00013843286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018470986,0.00016891042,0.00017650667,0.00090930547,0.00030880288,0.00045906432,0.00032281267,0.00026366606,0.0007112314],"category_scores_gemma":[0.00039954166,0.00012449894,0.00012948987,0.00048163367,0.00014894425,0.000264746,0.0006265945,0.00016234306,0.0002612471],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001701453,0.00008874357,0.94125336,0.000037105547,0.00009802065,0.0002629706,0.0004540983,0.00046636042,0.04696016,0.00020450467,0.0017194625,0.008285047],"study_design_scores_gemma":[0.000004862178,0.000010272285,0.99725443,0.000003875324,0.000006724001,0.00008258678,0.00006956063,0.00040990845,0.0009673382,0.000009668794,0.0011780171,0.0000028907325],"about_ca_topic_score_codex":0.01153452,"about_ca_topic_score_gemma":0.032740723,"teacher_disagreement_score":0.01153452,"about_ca_system_score_codex":0.00030237954,"about_ca_system_score_gemma":0.00019001213,"threshold_uncertainty_score":0.022934735},"labels":[],"label_agreement":null},{"id":"W3140539212","doi":"10.3847/1538-4357/abf3c4","title":"The JCMT BISTRO Survey: The Distribution of Magnetic Field Strengths toward the OMC-1 Region","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics; Queen's University","funders":"Science and Technology Facilities Council; Bureau of International Cooperation, Chinese Academy of Sciences; National Research Foundation of Korea","keywords":"Magnetic field; Polarization (electrochemistry); Mach number; Magnetic pressure; James Clerk Maxwell Telescope; Field (mathematics); Molecular cloud; Turbulence; Velocity dispersion","score_opus":0.013884627138971317,"score_gpt":0.24618605438429744,"score_spread":0.23230142724532613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3140539212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966382,0.00012061609,0.00017470702,0.000054863074,0.0000038921426,0.000011365156,0.0015880109,0.000066651766,0.00134154],"genre_scores_gemma":[0.99528813,0.00008619695,0.0008001273,0.000048551075,0.000028139806,0.000015666223,0.0033865245,0.00003160903,0.00031511317],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997181,0.000018520155,0.000012559156,0.00007348512,0.00011067431,0.000066590306],"domain_scores_gemma":[0.99866486,0.00010431776,0.0004978905,0.00013484717,0.00025650632,0.00034160924],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027349393,0.0002542703,0.00026045498,0.0024558206,0.00043182063,0.0005426125,0.00044190683,0.00033875668,0.0007589325],"category_scores_gemma":[0.0009230795,0.00015298919,0.00015604246,0.0015481338,0.0003123614,0.00031701033,0.0007767269,0.00023956716,0.00023206271],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014079882,0.000043415246,0.96484053,0.00004724894,0.00006358052,0.00025196178,0.00029105105,0.00068360264,0.018595897,0.00018817995,0.0022537136,0.012600115],"study_design_scores_gemma":[0.00000538062,0.000007780749,0.9977451,0.0000040803116,0.000006523143,0.000050640123,0.000043283864,0.00079565594,0.0004728834,0.000011646484,0.00085359265,0.0000033125466],"about_ca_topic_score_codex":0.031758826,"about_ca_topic_score_gemma":0.04658538,"teacher_disagreement_score":0.031758826,"about_ca_system_score_codex":0.0006930468,"about_ca_system_score_gemma":0.00038780295,"threshold_uncertainty_score":0.0631479},"labels":[],"label_agreement":null},{"id":"W3141763828","doi":"10.3847/1538-4357/abee7c","title":"Erratum: “Reinflation of Warm and Hot Jupiters” (2020, ApJ, 893, 36)","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Hot Jupiter; Astrophysics; Astronomy; Planet; Exoplanet","score_opus":0.007086233373601764,"score_gpt":0.21154397342213907,"score_spread":0.2044577400485373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3141763828","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00041259406,0.0011522444,0.00021151242,0.04927379,0.92169815,0.000028400842,0.003821833,0.00037253374,0.023029039],"genre_scores_gemma":[0.008225406,0.0042029256,0.002502452,0.10584169,0.14885218,0.00015468623,0.012172424,0.0014428329,0.71660537],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987643,0.00012313381,0.00019022277,0.00020561668,0.0005620993,0.00015461005],"domain_scores_gemma":[0.993711,0.0009107739,0.000367114,0.00042592388,0.0038310455,0.00075415097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017096618,0.0018185681,0.0009873671,0.0025067541,0.00432953,0.004126125,0.0019500925,0.004700105,0.08448361],"category_scores_gemma":[0.013058059,0.0006635042,0.0010568463,0.0016081608,0.0010741017,0.0028574294,0.0019194584,0.006416704,0.07554322],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000019090645,0.0000040274476,0.000057334266,0.000022081405,0.0000017009255,0.000054567787,0.000006356558,0.000010694339,0.00002943178,0.00021000483,0.99793553,0.0016492981],"study_design_scores_gemma":[0.000018969711,0.000016976728,0.0018110531,0.00010761925,0.000012485985,0.00011619559,0.00009574319,0.000059446596,0.0002016626,0.00055135164,0.9969894,0.000019154519],"about_ca_topic_score_codex":0.04136816,"about_ca_topic_score_gemma":0.06269139,"teacher_disagreement_score":0.08448361,"about_ca_system_score_codex":0.0026025292,"about_ca_system_score_gemma":0.0051151053,"threshold_uncertainty_score":0.28262585},"labels":[],"label_agreement":null},{"id":"W3144662244","doi":"10.3847/1538-4357/abea15","title":"SILVERRUSH X: Machine Learning-aided Selection of 9318 LAEs at z = 2.2, 3.3, 4.9, 5.7, 6.6, and 7.0 from the HSC SSP and CHORUS Survey Data","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Japan Society for the Promotion of Science; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; University of Tokyo; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; Max-Planck-Gesellschaft; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; Eötvös Loránd Tudományegyetem; Academia Sinica; Space Telescope Science Institute; Los Alamos National Laboratory; Johns Hopkins University; Princeton University; National Central University; Gordon and Betty Moore Foundation; Queen's University Belfast; National Aeronautics and Space Administration; Durham University; Japan Science and Technology Agency; Smithsonian Institution; National Science Foundation","keywords":"Reionization; Chorus; Convolutional neural network; Selection (genetic algorithm); COSMIC cancer database; Stars; Narrowband","score_opus":0.016984480456483323,"score_gpt":0.22843440562796954,"score_spread":0.21144992517148622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3144662244","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97702765,0.00015028402,0.00798623,0.00012939562,0.00002251756,0.00007797123,0.0064349435,0.005498527,0.0026725798],"genre_scores_gemma":[0.88473326,0.00009494553,0.050208703,0.00012625543,0.00008033429,0.000122001795,0.05949628,0.00060688367,0.004531298],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979097,0.000042185173,0.00001045026,0.000061350795,0.00005331073,0.000041752508],"domain_scores_gemma":[0.9993857,0.00011534549,0.0001168663,0.00015306113,0.00011648797,0.000112432106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00086474215,0.0003192051,0.00035619555,0.0020140172,0.0003310333,0.000476344,0.0005193712,0.00021760895,0.0027357333],"category_scores_gemma":[0.0009256468,0.00015158877,0.0004107628,0.0008288027,0.00013112028,0.0002529848,0.0006127587,0.00021873807,0.0013228819],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085241033,0.00047555173,0.5666704,0.00015993863,0.00030014015,0.0007706594,0.00025163175,0.028478198,0.04360552,0.0010876604,0.06741668,0.28993124],"study_design_scores_gemma":[0.00034656655,0.00030833087,0.5527816,0.000045861732,0.00013330505,0.00035286968,0.00021587736,0.38327488,0.031502135,0.00083588075,0.03015238,0.000050388095],"about_ca_topic_score_codex":0.0062576532,"about_ca_topic_score_gemma":0.012947026,"teacher_disagreement_score":0.0062576532,"about_ca_system_score_codex":0.00028406284,"about_ca_system_score_gemma":0.00043820057,"threshold_uncertainty_score":0.01244247},"labels":[],"label_agreement":null},{"id":"W3145322367","doi":"10.3847/1538-4357/aca485","title":"CHIME Discovery of a Binary Pulsar with a Massive Nondegenerate Companion","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; Herzberg Institute of Astrophysics; University of Toronto; Canadian Institute for Theoretical Astrophysics; University of British Columbia; McGill University","funders":"Canada Foundation for Innovation","keywords":"Binary pulsar; Pulsar; Astronomy; Physics; Astrophysics; Geology; Millisecond pulsar","score_opus":0.012930116515692489,"score_gpt":0.29434002052350133,"score_spread":0.28140990400780885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3145322367","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963664,0.00012104325,0.00035160215,0.00011679023,0.0000100728785,0.000012018235,0.000233518,0.00002084223,0.002767668],"genre_scores_gemma":[0.9975473,0.000080566635,0.00084071537,0.00005175384,0.0000074921845,0.00000393723,0.00042247085,0.0000027371564,0.0010429806],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992955,0.0000026005864,0.0000018427944,0.000020217849,0.000025437927,0.000020468486],"domain_scores_gemma":[0.99987435,0.0000097200045,0.0000200987,0.000016397791,0.000015857917,0.00006349886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012879694,0.00013805162,0.00014097581,0.00043017167,0.00076953525,0.0004005941,0.00019385165,0.0002662935,0.0007703457],"category_scores_gemma":[0.00025490482,0.00016020724,0.00006424427,0.00027033273,0.00037394426,0.00011759446,0.000578111,0.0003571378,0.00016470165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006253697,0.00011691119,0.667811,0.000062038795,0.00005130328,0.00734455,0.00062049954,0.00034401455,0.2674815,0.0022884414,0.0020325403,0.05122192],"study_design_scores_gemma":[0.00003252988,0.00019014734,0.9572378,0.000009927536,0.000022392729,0.005626725,0.00036297453,0.00080639205,0.019016344,0.0004400092,0.016239528,0.000015164343],"about_ca_topic_score_codex":0.01908102,"about_ca_topic_score_gemma":0.030823495,"teacher_disagreement_score":0.01908102,"about_ca_system_score_codex":0.0006339185,"about_ca_system_score_gemma":0.00044994187,"threshold_uncertainty_score":0.037939906},"labels":[],"label_agreement":null},{"id":"W3148438948","doi":"10.3847/1538-4357/abf2b2","title":"The Mass and Age Distribution of Halo White Dwarfs in the Canada–France Imaging Survey","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Halo; White dwarf; Galactic halo; Astrometry; Photometry (optics); Mass distribution; Spectral energy distribution; Stars; Stellar mass","score_opus":0.007079103872265072,"score_gpt":0.20616822796700102,"score_spread":0.19908912409473595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3148438948","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945532,0.00024698477,0.00008033776,0.00007959816,0.0000024265594,0.000006064857,0.0031362958,0.000025417214,0.0018697446],"genre_scores_gemma":[0.9947607,0.00014691797,0.00014787902,0.00003067515,0.0000028987786,0.0000053913345,0.003089369,0.00001025169,0.0018059132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995782,0.00003395487,0.00001339118,0.00008313801,0.00013895392,0.0001523981],"domain_scores_gemma":[0.99842024,0.00009018975,0.00025660277,0.000059684146,0.00079559203,0.0003776884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044424145,0.00029065422,0.00021059332,0.002882802,0.00065218314,0.0007147112,0.00043960003,0.00022470734,0.0019246761],"category_scores_gemma":[0.0010990398,0.00013248365,0.00019631363,0.0015078756,0.00036077623,0.00022205825,0.0003394474,0.000151051,0.00038858605],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042205105,0.00000604319,0.9945515,0.0000047229964,0.00002116581,0.0000482623,0.00034522032,0.00010750587,0.0010043792,0.00009551016,0.00096984074,0.0028036279],"study_design_scores_gemma":[0.0000010201248,0.0000052371865,0.99844307,0.0000030259362,0.0000032741893,0.000033840224,0.00022688799,0.00010700242,0.00012211625,0.000004784794,0.0010456134,0.0000041625394],"about_ca_topic_score_codex":0.9342869,"about_ca_topic_score_gemma":0.9513363,"teacher_disagreement_score":0.9342869,"about_ca_system_score_codex":0.0057207216,"about_ca_system_score_gemma":0.0025628924,"threshold_uncertainty_score":0.13220018},"labels":[],"label_agreement":null},{"id":"W3148571830","doi":"10.3847/1538-4357/abe466","title":"Rapidly Declining Hostless Type Ia Supernova KSP-OT-201509b from the KMTNet Supernova Program: Transitional Nature and Constraint on <sup>56</sup>Ni Distribution and Progenitor Type","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Ejecta; Supernova; Light curve; Luminosity; Redshift; Galaxy; Type (biology); Stars","score_opus":0.013582007724397301,"score_gpt":0.2638366772546301,"score_spread":0.2502546695302328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3148571830","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984054,0.0000594079,0.000249065,0.000012903471,0.0000063864513,0.000008203337,0.00034215147,0.000014783551,0.0009016842],"genre_scores_gemma":[0.9982994,0.000028532144,0.00024094566,0.000013127758,0.000003842557,0.000003672956,0.0011443003,0.000008598793,0.00025769358],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988914,0.0000067803103,0.000011251807,0.000034198678,0.000030891624,0.0000278495],"domain_scores_gemma":[0.99940264,0.000036962625,0.00013935893,0.00007671956,0.00006922196,0.0002750149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002840791,0.0002598535,0.00030755828,0.0007415112,0.00047888464,0.00070436706,0.00033577628,0.00015329555,0.00082031195],"category_scores_gemma":[0.00034863185,0.00012246174,0.00029098944,0.0003916393,0.00036255945,0.00017445415,0.0006690463,0.00037901185,0.00029355526],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009361485,0.00009421914,0.92527217,0.000037124904,0.00008400917,0.0015145566,0.00014624948,0.00047548703,0.06268233,0.00066717016,0.00029506744,0.0077954363],"study_design_scores_gemma":[0.000018009116,0.00015739523,0.9894518,0.000009068759,0.00003427805,0.0016756546,0.00010964396,0.00066442485,0.006261428,0.000156671,0.0014518395,0.000009666282],"about_ca_topic_score_codex":0.0036968621,"about_ca_topic_score_gemma":0.0056608934,"teacher_disagreement_score":0.0036968621,"about_ca_system_score_codex":0.00031104047,"about_ca_system_score_gemma":0.0002475258,"threshold_uncertainty_score":0.007350683},"labels":[],"label_agreement":null},{"id":"W3149658418","doi":"10.3847/1538-4357/abf2b6","title":"Magnetic Fields in Massive Star-forming Regions (MagMaR). I. Linear Polarized Imaging of the Ultracompact H ii Region G5.89–0.39","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Japan Society for the Promotion of Science; Consejo Nacional de Ciencia y Tecnología; Japan Society of Applied Physics","keywords":"Star (game theory); Physics; Magnetic field; Astronomy; Astrophysics; Geology; Nuclear magnetic resonance; Quantum mechanics","score_opus":0.0104527910502784,"score_gpt":0.23841539417437763,"score_spread":0.22796260312409922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3149658418","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983216,0.000093223076,0.00016897786,0.00002188836,0.0000013610123,0.0000032070614,0.00019330811,0.000020340472,0.0011761996],"genre_scores_gemma":[0.999286,0.00003407709,0.0003506838,0.000016268212,0.000006202775,0.0000018806551,0.00018527525,0.0000040270024,0.00011570678],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997175,0.0000025015038,9.918651e-7,0.0000082158,0.000007499615,0.000009013039],"domain_scores_gemma":[0.9999217,0.000006812447,0.00003533059,0.000005245448,0.000009746549,0.00002120688],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007095326,0.00009441579,0.00008653479,0.00037737846,0.00018660704,0.00018667661,0.00017450024,0.00012120648,0.00062223943],"category_scores_gemma":[0.000107386324,0.00009078543,0.00008864799,0.00022884461,0.00012384522,0.00009933689,0.00021690236,0.00012689074,0.00019103818],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004150714,0.00006655795,0.5125886,0.00007032449,0.00006621323,0.00094691303,0.00073228724,0.00043312396,0.46513703,0.00035698924,0.00070976734,0.018477077],"study_design_scores_gemma":[0.0000046405517,0.000022770519,0.9970391,0.0000027946835,0.000005601125,0.00019826936,0.00007395724,0.0002394835,0.0019036508,0.000041262014,0.0004669125,0.0000016263822],"about_ca_topic_score_codex":0.0030462402,"about_ca_topic_score_gemma":0.0035533737,"teacher_disagreement_score":0.0030462402,"about_ca_system_score_codex":0.0001932701,"about_ca_system_score_gemma":0.0000457117,"threshold_uncertainty_score":0.006057024},"labels":[],"label_agreement":null},{"id":"W3151173739","doi":"10.3847/1538-4357/ac230b","title":"The XFaster Power Spectrum and Likelihood Estimator for the Analysis of Cosmic Microwave Background Maps","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"British Antarctic Survey; British Columbia Knowledge Development Fund; Norges Forskningsråd; Science and Technology Facilities Council; University of Toronto; Canadian Space Agency; Inyuvesi Yakwazulu-Natali; UK Research and Innovation; University of Texas at Austin; Princeton University; Science Mission Directorate; Government of Ontario; National Aeronautics and Space Administration; National Science Foundation; Compute Canada; University of Chicago; Vetenskapsrådet","keywords":"Estimator; Monte Carlo method; Cosmic microwave background; Algorithm; Planck; Markov chain Monte Carlo; Physics; Spectral density; Hybrid Monte Carlo; Statistical physics; Computer science; Statistics; Astrophysics; Mathematics; Anisotropy; Optics","score_opus":0.009656767850124209,"score_gpt":0.25872747508763216,"score_spread":0.24907070723750796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3151173739","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0077151326,0.00011540736,0.98800194,0.000078969686,0.000018493147,0.000026881,0.0004179712,0.0027152603,0.0009099707],"genre_scores_gemma":[0.21784036,0.00019854035,0.77263546,0.00011306848,0.00010213678,0.0002599433,0.0027072846,0.002831261,0.0033120164],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990089,0.00045449732,0.000039360577,0.00011657684,0.0003199118,0.000060739778],"domain_scores_gemma":[0.99627435,0.0025477537,0.00020583949,0.00048141787,0.0004046535,0.000086064254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029233664,0.0008023802,0.000520856,0.0021155544,0.00048505134,0.0012100927,0.0016312754,0.0004977251,0.008126115],"category_scores_gemma":[0.019242715,0.0005000786,0.0009044756,0.0012157265,0.00080858043,0.001500795,0.001771619,0.00088250043,0.0016081057],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002843197,0.00009482286,0.014355924,0.00030373642,0.000319126,0.00034538537,0.00022385178,0.44755378,0.005257678,0.12525284,0.01967243,0.386336],"study_design_scores_gemma":[0.00002865224,0.000013890046,0.0021213007,0.00001979309,0.000009369498,0.000079954036,0.00001569109,0.9459449,0.0017795154,0.045835905,0.0041283984,0.000022686569],"about_ca_topic_score_codex":0.0066560498,"about_ca_topic_score_gemma":0.0044834632,"teacher_disagreement_score":0.008126115,"about_ca_system_score_codex":0.0006721734,"about_ca_system_score_gemma":0.0011771136,"threshold_uncertainty_score":0.027184546},"labels":[],"label_agreement":null},{"id":"W3151304702","doi":"10.3847/1538-4357/abf4c8","title":"Magnetic Properties of Star-forming Dense Cores","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Zeeman effect; Magnetic field; Polarization (electrochemistry); Amplitude; Field strength; Field (mathematics); Range (aeronautics); Dispersion (optics)","score_opus":0.015509102442794038,"score_gpt":0.22234095048502675,"score_spread":0.2068318480422327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3151304702","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99879044,0.00007411684,0.000059065515,0.000006027734,9.397577e-7,0.0000016497523,0.00021957833,0.0000075575595,0.0008406756],"genre_scores_gemma":[0.99898285,0.00002097687,0.00005419619,0.0000046387254,0.0000029488713,0.0000013170131,0.00066005014,0.0000030779372,0.00026983544],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995065,0.0000034919976,0.0000030046742,0.0000100424095,0.000012127767,0.000020678699],"domain_scores_gemma":[0.9994679,0.00006712566,0.00014958027,0.00003070202,0.0001029029,0.00018182913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000119519114,0.00015155408,0.00017534888,0.0006630935,0.00022319684,0.00033528748,0.00013512064,0.000087394925,0.0014432109],"category_scores_gemma":[0.0005908061,0.00009558038,0.000071908726,0.0003794882,0.00018447015,0.00012710653,0.0003234553,0.0001221294,0.0002745112],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004923813,0.000057903355,0.9395274,0.000042751806,0.000076540964,0.000337181,0.00026223995,0.0017326532,0.047045454,0.0005494807,0.0010389949,0.0088369865],"study_design_scores_gemma":[0.00001596605,0.000066083965,0.99428284,0.0000052314,0.000009348685,0.00016595566,0.0001219448,0.0013371729,0.002829448,0.00016227418,0.0009993629,0.0000044175063],"about_ca_topic_score_codex":0.00495664,"about_ca_topic_score_gemma":0.0038120938,"teacher_disagreement_score":0.00495664,"about_ca_system_score_codex":0.00022868495,"about_ca_system_score_gemma":0.000089497626,"threshold_uncertainty_score":0.009855568},"labels":[],"label_agreement":null},{"id":"W3152540566","doi":"10.3847/1538-4357/abebe4","title":"The Intrinsic Scatter of Galaxy Scaling Relations","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Scaling; Galaxy; Photometry (optics); Angular momentum; Stellar mass; Galaxy formation and evolution; Cosmology; Stars","score_opus":0.006995006228567762,"score_gpt":0.21100034637963322,"score_spread":0.20400534015106545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3152540566","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78437006,0.0017773963,0.2014369,0.00014395462,0.000031710788,0.000023727462,0.002342546,0.0009073772,0.008966324],"genre_scores_gemma":[0.9889324,0.000250528,0.00945303,0.000017354569,0.000017167176,0.000010665688,0.0009955973,0.00006033575,0.00026293623],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99751735,0.0006953052,0.00020043684,0.0005821222,0.00090919435,0.000095534146],"domain_scores_gemma":[0.9844626,0.008472582,0.001632957,0.0032179037,0.002051255,0.00016275248],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0035612162,0.00036576221,0.00053840596,0.002960393,0.00029301224,0.001703865,0.00044140985,0.00021915516,0.0012048199],"category_scores_gemma":[0.019227011,0.00037218272,0.00046931658,0.0018930373,0.0007860359,0.0010397126,0.0008832988,0.0005752466,0.0003332314],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000118549884,0.000045740813,0.64509386,0.00023407514,0.00073418714,0.0001536126,0.001048243,0.10209584,0.012499794,0.04130658,0.002463833,0.19420575],"study_design_scores_gemma":[0.000013159548,0.000071878545,0.62065035,0.00013230654,0.00011808013,0.00048240385,0.00025631432,0.29489738,0.008997646,0.064710304,0.009533801,0.00013643273],"about_ca_topic_score_codex":0.0031035864,"about_ca_topic_score_gemma":0.0031945854,"teacher_disagreement_score":0.0035612162,"about_ca_system_score_codex":0.0005819277,"about_ca_system_score_gemma":0.00029012046,"threshold_uncertainty_score":0.018833697},"labels":[],"label_agreement":null},{"id":"W3152858534","doi":"10.3847/1538-4357/abd17b","title":"Constraints on the Mass Accretion Rate onto the Supermassive Black Hole of Cygnus A Using the Submillimeter Array","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Astrophysics; Supermassive black hole; Accretion (finance); Polarization (electrochemistry); Faraday effect; Outflow; Submillimeter Array; Astronomy; Magnetic field; Galaxy; Star formation","score_opus":0.026047068247978568,"score_gpt":0.2466296560844151,"score_spread":0.22058258783643653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3152858534","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958533,0.00032167818,0.0016226264,0.000047378617,0.000006505089,0.000004649266,0.00019378179,0.000034782843,0.0019152353],"genre_scores_gemma":[0.9991228,0.000050693947,0.0006208742,0.000011751189,0.000007756387,0.0000042511833,0.00009308336,0.000003515285,0.00008540042],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999006,0.000018775321,0.000003947926,0.000028856346,0.000023973498,0.00002391251],"domain_scores_gemma":[0.99946827,0.00019012007,0.00019030891,0.00005528843,0.00004756784,0.00004856287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039432745,0.00033726697,0.00026780053,0.0008494488,0.00023870051,0.00041862228,0.00024365298,0.00022836967,0.0008970564],"category_scores_gemma":[0.00093543925,0.00020232612,0.00020143163,0.0003006427,0.00017775582,0.00026625133,0.00030806835,0.0001649053,0.0002303483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003377015,0.00003524818,0.62549466,0.00006715859,0.00011502773,0.00035474144,0.00022927736,0.0051110787,0.3505796,0.0025176883,0.00040349067,0.014754347],"study_design_scores_gemma":[0.00001754576,0.00007610099,0.96216005,0.0000215326,0.00006235878,0.00022160583,0.00010424732,0.012776835,0.0220758,0.0010131642,0.0014526851,0.000018057357],"about_ca_topic_score_codex":0.001897797,"about_ca_topic_score_gemma":0.0027433035,"teacher_disagreement_score":0.001897797,"about_ca_system_score_codex":0.00033715813,"about_ca_system_score_gemma":0.00016279863,"threshold_uncertainty_score":0.0037735105},"labels":[],"label_agreement":null},{"id":"W3152861303","doi":"10.3847/1538-4357/ac1dac","title":"Capturing the Physics of MaNGA Galaxies with Self-supervised Machine Learning","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Ministerio de Ciencia, Innovación y Universidades; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; European Commission; Ministerio de Ciencia e Innovación; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Agencia Estatal de Investigación; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Galaxy; Physics; Perspective (graphical); Field (mathematics); Population; Astrophysics; Cluster analysis; Visualization; Computer science; Artificial intelligence; Mathematics","score_opus":0.013635775021015015,"score_gpt":0.2419006804484705,"score_spread":0.22826490542745548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3152861303","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.43012533,0.00044992182,0.5618334,0.000537032,0.000052167536,0.000060011145,0.0013549037,0.003951082,0.0016361075],"genre_scores_gemma":[0.85762644,0.00010867041,0.13904625,0.00009914163,0.000085107225,0.00005931523,0.0019593348,0.00021754998,0.00079830043],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997832,0.00007860854,0.000009577732,0.00006130593,0.000040301227,0.000027074413],"domain_scores_gemma":[0.998533,0.00062926696,0.00020851161,0.00033190634,0.00017639536,0.000120907775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007269401,0.0003953537,0.00042046598,0.001389401,0.0002750939,0.0008915764,0.0009683112,0.0005340274,0.00084567076],"category_scores_gemma":[0.0026248817,0.0002669557,0.00063802465,0.00067846203,0.00066363724,0.0009435725,0.00090416713,0.0006462516,0.00033788328],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026191716,0.0003303873,0.065097965,0.0002415355,0.00025315408,0.00020013173,0.00047545446,0.7405674,0.018505003,0.017043576,0.007049325,0.14997418],"study_design_scores_gemma":[0.0000039123356,0.0000065097215,0.0030879653,0.000004066444,0.0000028774093,0.000011183304,0.000013114555,0.9899997,0.0008492865,0.005607892,0.0004083604,0.0000049885875],"about_ca_topic_score_codex":0.0032083108,"about_ca_topic_score_gemma":0.00313768,"teacher_disagreement_score":0.0032083108,"about_ca_system_score_codex":0.0005397929,"about_ca_system_score_gemma":0.00039945176,"threshold_uncertainty_score":0.0063792467},"labels":[],"label_agreement":null},{"id":"W3152864662","doi":"10.3847/1538-4357/ac32cd","title":"Validation of the HERA Phase I Epoch of Reionization 21 cm Power Spectrum Software Pipeline","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Gordon and Betty Moore Foundation; Science and Technology Facilities Council; National Science Foundation","keywords":"Reionization; Physics; HERA; Pipeline (software); Astronomy; Astrophysics; Spectral density; Epoch (astronomy); Phase (matter); Stars; Galaxy; Particle physics; Redshift; Telecommunications","score_opus":0.0078057853878644575,"score_gpt":0.23020320178833076,"score_spread":0.2223974164004663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3152864662","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.817948,0.00011066326,0.13200858,0.00097562664,0.00020279127,0.00042830274,0.0048923753,0.021600023,0.021833716],"genre_scores_gemma":[0.94029176,0.00003132245,0.051148802,0.00022698002,0.000025156965,0.00025351535,0.004024132,0.0024215647,0.0015768463],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99807656,0.00063134293,0.000098243865,0.00027850803,0.000691082,0.00022423119],"domain_scores_gemma":[0.99112064,0.0031380916,0.000596895,0.0025790476,0.0021372105,0.0004281679],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0057278266,0.0007774704,0.0004734094,0.00079143536,0.0007099789,0.0015310826,0.0022496232,0.00073538534,0.003046395],"category_scores_gemma":[0.016024094,0.0005750382,0.0008573887,0.00060261594,0.00068611716,0.0013898886,0.0015892613,0.0015084328,0.0015564865],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019306594,0.0005581614,0.085075736,0.00019103725,0.0003557707,0.0005241799,0.0013627326,0.77349037,0.031028079,0.020345742,0.017033879,0.068103746],"study_design_scores_gemma":[0.00031275852,0.00044134443,0.016729929,0.000053966585,0.0000462504,0.000103029895,0.0001635262,0.92314565,0.043062042,0.005087673,0.010737001,0.00011680897],"about_ca_topic_score_codex":0.007284904,"about_ca_topic_score_gemma":0.0034504724,"teacher_disagreement_score":0.007284904,"about_ca_system_score_codex":0.0019006017,"about_ca_system_score_gemma":0.001447701,"threshold_uncertainty_score":0.030292034},"labels":[],"label_agreement":null},{"id":"W3154025755","doi":"10.3847/1538-4357/abf3c2","title":"Star Formation Histories from Spectral Energy Distributions and Color–magnitude Diagrams Agree: Evidence for Synchronized Star Formation in Local Volume Dwarf Galaxies over the Past 3 Gyr","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"High Energy Physics; Office of Science; U.S. Department of Energy","keywords":"Star formation; Galaxy; Dwarf galaxy; Local Group; Stars; Dwarf spheroidal galaxy; Galaxy formation and evolution","score_opus":0.010852104031487694,"score_gpt":0.2204024986532996,"score_spread":0.2095503946218119,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154025755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989334,0.0000333994,0.0004165265,0.000006964303,7.461989e-7,0.0000022795673,0.000289957,0.000020204006,0.00029646],"genre_scores_gemma":[0.99923587,0.000010932896,0.00031246088,0.0000017894604,0.0000012955906,0.0000012899698,0.00036893002,0.000004110606,0.00006337806],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998596,0.000023639104,0.000011657517,0.000048218433,0.000037877595,0.000019019968],"domain_scores_gemma":[0.99849594,0.0002809858,0.0005694786,0.00022746419,0.0002083544,0.00021784518],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042318564,0.00010367581,0.00017969546,0.0010495345,0.00014211197,0.00042450527,0.00022635625,0.00011778827,0.0006741417],"category_scores_gemma":[0.002364073,0.00009888117,0.00019144207,0.0007429014,0.00021450597,0.00030491923,0.00036670858,0.00012285767,0.00014926458],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004219292,0.000007798915,0.9889949,0.000005976215,0.0000287212,0.000022816204,0.00016345,0.00039971672,0.0049841497,0.000055805667,0.000052612744,0.0052419],"study_design_scores_gemma":[4.7394298e-7,0.000013085268,0.99840945,0.0000010745632,0.0000041634594,0.000031774754,0.00006132781,0.00092308666,0.00044965497,0.00002113343,0.00008337552,0.000001393211],"about_ca_topic_score_codex":0.007302806,"about_ca_topic_score_gemma":0.012782946,"teacher_disagreement_score":0.007302806,"about_ca_system_score_codex":0.00025014143,"about_ca_system_score_gemma":0.00010455943,"threshold_uncertainty_score":0.014520645},"labels":[],"label_agreement":null},{"id":"W3154141723","doi":"10.3847/1538-4357/ac1a10","title":"New Families in our Solar Neighborhood: Applying Gaussian Mixture Models for Objective Classification of Structures in the Milky Way and in Simulations","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council; Science Mission Directorate; Ames Research Center; Office of Science; Nuclear Safety and Security Commission; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Max-Planck-Institut für Astronomie; University of New South Wales; Government of Canada; University of Toronto; Carnegie Mellon University; Aspen Center for Physics; Carnegie Institution of Washington; Space Telescope Science Institute; Flatiron Health; Alfred P. Sloan Foundation; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; U.S. Department of Energy; University of Utah; Research Corporation for Science Advancement","keywords":"Milky Way; Astrophysics; Physics; Thin disk; Galaxy; Stars; Halo; Thick disk; Bulge; Galaxy formation and evolution; Mixture model; Astronomy; Artificial intelligence; Computer science","score_opus":0.02625135067880026,"score_gpt":0.3042944549212648,"score_spread":0.27804310424246453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154141723","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92558855,0.00010416241,0.072023384,0.00027981313,0.000012992621,0.00007657577,0.00049333746,0.00050868635,0.00091245637],"genre_scores_gemma":[0.96474165,0.000043565247,0.033558387,0.0000557327,0.000013883714,0.000070696515,0.0009094557,0.00011944968,0.00048711474],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99937856,0.00030697623,0.000020859594,0.0001692355,0.00006386738,0.000060546492],"domain_scores_gemma":[0.99667394,0.0021947639,0.00024720287,0.0004233172,0.00026405056,0.00019669486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003328516,0.0005027091,0.0007493626,0.0016392252,0.00060669443,0.0014316672,0.0016599646,0.0011004097,0.0012467026],"category_scores_gemma":[0.010974498,0.00046227055,0.0011597561,0.0009258303,0.0006915794,0.001635592,0.0013530956,0.0010118826,0.00020462803],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001133353,0.000072674724,0.041143063,0.0000140962065,0.00009568624,0.00005064624,0.00023884799,0.94093776,0.00031089032,0.0055983267,0.0005931332,0.010831597],"study_design_scores_gemma":[0.0000063020675,0.000006039176,0.0013235003,0.0000023310604,0.000003831883,0.000003949039,0.0000251852,0.99687636,0.000087539156,0.0015548943,0.00010629842,0.000003875799],"about_ca_topic_score_codex":0.03963522,"about_ca_topic_score_gemma":0.031309683,"teacher_disagreement_score":0.03963522,"about_ca_system_score_codex":0.0018503423,"about_ca_system_score_gemma":0.00058877375,"threshold_uncertainty_score":0.07880902},"labels":[],"label_agreement":null},{"id":"W3154375570","doi":"10.3847/1538-4357/ac0d5a","title":"Search for Neutrinos in Coincidence with Gravitational Wave Events from the LIGO–Virgo O3a Observing Run with the Super-Kamiokande Detector","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg; British Columbia Institute of Technology; TRIUMF; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Culture, Sports, Science and Technology; Japan Society for the Promotion of Science; Horizon 2020 Framework Programme; Kerman Neuroscience Research Center, Kerman University of Medical Sciences; Science and Technology Facilities Council; National Research Foundation; U.S. Department of Energy; European Commission; Western Canada Research Grid; National Natural Science Foundation of China; National Science Foundation; Compute Canada; National Research Foundation of Korea; Narodowym Centrum Nauki","keywords":"Gravitational wave; Neutrino; Coincidence; Detector; Equipartition theorem; Sky; Event (particle physics); Gravitational-wave observatory","score_opus":0.018962190964163208,"score_gpt":0.23508293796549012,"score_spread":0.2161207470013269,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154375570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965857,0.000063922016,0.001847251,0.000017603903,0.0000063612442,0.000017292066,0.00071118,0.00007177889,0.0006788916],"genre_scores_gemma":[0.9973455,0.000014258483,0.0011222885,0.000008377367,0.000008329837,0.000008659861,0.0012831296,0.000025228575,0.0001842991],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982591,0.00039421592,0.00011303323,0.00048707335,0.00047650843,0.00027008593],"domain_scores_gemma":[0.9963701,0.0013697232,0.0010002672,0.00047834511,0.00027084502,0.0005108646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023321984,0.00034643474,0.0004712685,0.002043175,0.0006020657,0.0010868924,0.0004501791,0.00041544903,0.002469896],"category_scores_gemma":[0.00381606,0.00027736244,0.0007579991,0.0021239219,0.00030532447,0.00032752746,0.0015772434,0.00041084894,0.00035726427],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016195175,0.000099345176,0.96319157,0.000048534905,0.0003751594,0.0006691072,0.00021233632,0.0006894873,0.02384381,0.00057612144,0.00034730902,0.008327734],"study_design_scores_gemma":[0.0001017134,0.00039094093,0.9735301,0.000014839073,0.00034967702,0.0009197216,0.00022612119,0.0077188285,0.014138265,0.00063468807,0.0019447041,0.0000304433],"about_ca_topic_score_codex":0.0023280592,"about_ca_topic_score_gemma":0.0030345598,"teacher_disagreement_score":0.002469896,"about_ca_system_score_codex":0.0002965395,"about_ca_system_score_gemma":0.00049047574,"threshold_uncertainty_score":0.012333989},"labels":[],"label_agreement":null},{"id":"W3154531344","doi":"10.3847/1538-4357/ac2307","title":"The Atacama Cosmology Telescope: A Search for Planet 9","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Flatiron Health; Institut Périmètre de physique théorique; Science and Technology Facilities Council; University of Toronto; European Commission; Government of Ontario; Industry Canada; National Science Foundation; Compute Canada; University of Pennsylvania; Princeton University; Ministry of Colleges and Universities; Government of Canada","keywords":"Planet; Physics; Astrophysics; Sky; Planetary mass; Minimum mass; Astronomy; Cosmology; Flux (metallurgy); Exoplanet","score_opus":0.02098088904619033,"score_gpt":0.2665699289310224,"score_spread":0.24558903988483205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154531344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9297362,0.0008982151,0.013761131,0.0011314751,0.00009614984,0.0001990165,0.020815503,0.00123955,0.03212266],"genre_scores_gemma":[0.9399854,0.00018443409,0.03542719,0.0003300859,0.00010143483,0.00006805182,0.019995252,0.00014646538,0.0037617951],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995426,0.00006313998,0.000017677196,0.0000853779,0.00020837458,0.00008283479],"domain_scores_gemma":[0.9990683,0.00011347732,0.00018374238,0.00017191705,0.000185325,0.00027722132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007760382,0.00020432252,0.00033222997,0.0018610477,0.0009917326,0.00072804594,0.00063290464,0.00039511218,0.0032090885],"category_scores_gemma":[0.00088531466,0.00021104458,0.00035846382,0.0021724105,0.00020064725,0.00036800522,0.00078477926,0.00045789935,0.0013294776],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038598932,0.00022820375,0.8367716,0.0001717412,0.00025885098,0.0009253669,0.00051010976,0.0036152783,0.031477038,0.0026979493,0.04099517,0.08196262],"study_design_scores_gemma":[0.00007148831,0.000099752535,0.933875,0.00004737262,0.00007838916,0.00044528933,0.00033043112,0.015428538,0.0051626866,0.0009257988,0.043499235,0.00003596846],"about_ca_topic_score_codex":0.01735586,"about_ca_topic_score_gemma":0.027190935,"teacher_disagreement_score":0.01735586,"about_ca_system_score_codex":0.0005242127,"about_ca_system_score_gemma":0.000784417,"threshold_uncertainty_score":0.03450966},"labels":[],"label_agreement":null},{"id":"W3154547568","doi":"10.3847/1538-4357/abf92b","title":"Robust Assessment of Clustering Methods for Fast Radio Transient Candidates","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Cluster analysis; Metric (unit); Transient (computer programming); Set (abstract data type); Noise (video); Benchmark (surveying); Correlation clustering; Visualization; Measure (data warehouse)","score_opus":0.025238591528597434,"score_gpt":0.3143561729717739,"score_spread":0.28911758144317645,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154547568","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.18343765,0.00079140865,0.80853057,0.00030560637,0.00014937272,0.0002963964,0.00065906235,0.0035714835,0.0022584656],"genre_scores_gemma":[0.62599194,0.0001660645,0.36987028,0.00007534315,0.000052922634,0.00015330096,0.0016989006,0.0006837075,0.0013076032],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9959376,0.0011779047,0.0003357294,0.00094319944,0.0013275709,0.00027795622],"domain_scores_gemma":[0.98220736,0.006852192,0.0018991682,0.002343503,0.0061964015,0.0005013063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0088247,0.0013449936,0.00090968725,0.005728435,0.0013408905,0.0027439543,0.0020780733,0.0017259406,0.0015332774],"category_scores_gemma":[0.034212254,0.0003936546,0.00097379467,0.0026692066,0.0007721478,0.0017532278,0.0020778398,0.00089893705,0.0009153416],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014846467,0.00036326444,0.039209604,0.00047263489,0.0008227882,0.00014968691,0.00051305356,0.5354111,0.035691004,0.01118989,0.0067391624,0.36795315],"study_design_scores_gemma":[0.00003684309,0.00016172572,0.009743413,0.000031500465,0.00004370496,0.00010476938,0.00019016497,0.9662475,0.018348863,0.0036593243,0.0013741908,0.000058039645],"about_ca_topic_score_codex":0.0068809255,"about_ca_topic_score_gemma":0.005380652,"teacher_disagreement_score":0.0088247,"about_ca_system_score_codex":0.0018258726,"about_ca_system_score_gemma":0.001518584,"threshold_uncertainty_score":0.04667008},"labels":[],"label_agreement":null},{"id":"W3154970985","doi":"10.3847/1538-4357/abf6d4","title":"Multiwavelength Follow-up of FRB180309","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"National Science Foundation","keywords":"Physics; Redshift; Astrophysics; Luminosity; Galaxy; Flux (metallurgy); Telescope; Chemistry","score_opus":0.008890288784217626,"score_gpt":0.21626063950104865,"score_spread":0.20737035071683102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3154970985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99417263,0.0002651751,0.00061823515,0.00018719099,0.00001556643,0.000026523818,0.00082744664,0.000057809113,0.0038294785],"genre_scores_gemma":[0.99684924,0.00004037348,0.0006895532,0.000120778735,0.000010145184,0.000013809732,0.00073430943,0.000012485694,0.0015294073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981004,0.000010096402,0.0000073287124,0.000055105847,0.000045986577,0.00007145291],"domain_scores_gemma":[0.99933785,0.00004956813,0.00019729133,0.00007641915,0.00013584111,0.00020305438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002775963,0.00022524103,0.00037316416,0.000990734,0.0010839466,0.0003314309,0.0003168783,0.00047085088,0.0025165407],"category_scores_gemma":[0.00038089027,0.00017944857,0.00032767552,0.000366782,0.00022252752,0.00034138747,0.00061155064,0.00063063786,0.0011000282],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004000282,0.00022917638,0.8722772,0.00005505313,0.00006813699,0.0027191285,0.00086662953,0.00030907965,0.08871752,0.00020895644,0.0030411493,0.031108065],"study_design_scores_gemma":[0.0000048404186,0.000093918614,0.9950806,0.0000061329065,0.000012082821,0.0006194557,0.00016671025,0.000132763,0.0018006184,0.00005259612,0.002023602,0.0000067556102],"about_ca_topic_score_codex":0.016949758,"about_ca_topic_score_gemma":0.04342947,"teacher_disagreement_score":0.016949758,"about_ca_system_score_codex":0.00066519977,"about_ca_system_score_gemma":0.00024197291,"threshold_uncertainty_score":0.033702254},"labels":[],"label_agreement":null},{"id":"W3155821239","doi":"10.3847/1538-4357/ac1675","title":"Evidence of a Dwarf Galaxy Stream Populating the Inner Milky Way Halo","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Institut sur la Nutrition et les Aliments Fonctionnels; National Development and Reform Commission; Chinese Academy of Sciences; Agence Nationale de la Recherche; Johns Hopkins University; Yale University; Vanderbilt University; New Mexico State University; University of Portsmouth; University of Washington; Ohio State University; Princeton University; College of Engineering, Michigan State University; Harvard University; York University","keywords":"Physics; Astrophysics; Milky Way; Dwarf galaxy; Globular cluster; Metallicity; Dwarf spheroidal galaxy; Galaxy; Galactic halo; Astronomy; Stellar population; Population; Velocity dispersion; Halo; Interacting galaxy; Star formation","score_opus":0.03114056818784054,"score_gpt":0.26592173596619767,"score_spread":0.23478116777835714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3155821239","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99930644,0.00006463757,0.00009123759,0.000009543611,0.0000014879412,0.0000033334677,0.000107506516,0.00002268663,0.0003931943],"genre_scores_gemma":[0.9990941,0.000059796184,0.00025198696,0.000012025329,0.000008399645,0.0000032013745,0.00041973646,0.000006471076,0.00014424279],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987483,0.000008257387,0.000011063514,0.000030721436,0.000039780192,0.000035293517],"domain_scores_gemma":[0.999286,0.00005590526,0.0002779749,0.000068496556,0.00010348986,0.00020821522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017964047,0.00018347432,0.00026482574,0.001548671,0.0004043001,0.0007099549,0.0002711541,0.00021846485,0.0010469796],"category_scores_gemma":[0.0005573119,0.0001446083,0.00016955312,0.0007495222,0.00032237687,0.00030949787,0.0007182286,0.00014659305,0.00034731303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007128523,0.000019211866,0.97698694,0.000020863175,0.00002078927,0.0003546863,0.0002402467,0.00009432147,0.015928723,0.00019291483,0.00017344634,0.005896557],"study_design_scores_gemma":[0.0000073973874,0.00004102981,0.9953815,0.0000074752334,0.000017658655,0.00036562845,0.00016938336,0.0005756467,0.0023262068,0.00009966408,0.0010046822,0.000003878085],"about_ca_topic_score_codex":0.002268104,"about_ca_topic_score_gemma":0.0039061718,"teacher_disagreement_score":0.002268104,"about_ca_system_score_codex":0.0002934383,"about_ca_system_score_gemma":0.00021303214,"threshold_uncertainty_score":0.004509747},"labels":[],"label_agreement":null},{"id":"W3156036410","doi":"10.3847/1538-4357/ac2a35","title":"A Model of Spectral Line Broadening in Signal Forecasts for Line-intensity Mapping Experiments","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Astronomical Sciences","keywords":"Physics; Intensity mapping; Intensity (physics); Attenuation; Line (geometry); Context (archaeology); Computational physics; Spectral density; Amplitude; Spectral line; Hydrogen line; Noise (video); Optics; Astrophysics; Statistics; Mathematics; Quantum mechanics; Computer science; Geometry","score_opus":0.032692626871168244,"score_gpt":0.25434887884305285,"score_spread":0.2216562519718846,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3156036410","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4491717,0.00017749342,0.53978205,0.0020882417,0.000066291184,0.00020664703,0.00057867996,0.00087005005,0.0070588742],"genre_scores_gemma":[0.97392255,0.000091353955,0.021227552,0.00015825623,0.000044562632,0.00010899198,0.0002480044,0.00010346172,0.004095169],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9988053,0.0004474123,0.000049255945,0.00033918413,0.00017806645,0.00018066785],"domain_scores_gemma":[0.9872607,0.008999592,0.001588798,0.00063482224,0.0009724203,0.0005435319],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0054934304,0.0008403739,0.00072389183,0.00097247027,0.00068788853,0.0016584204,0.0026191107,0.0025362486,0.0031352546],"category_scores_gemma":[0.025894005,0.0007688818,0.00066828117,0.0007459657,0.0016008316,0.0029885904,0.0012694382,0.0017005944,0.000686246],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010335824,0.00004321703,0.004319701,0.000030287336,0.00002067088,0.00018135698,0.00021098436,0.95453846,0.0023610557,0.031632643,0.0005871006,0.005971224],"study_design_scores_gemma":[0.0000071528266,0.000015887063,0.0009578302,0.000004741153,0.0000039280353,0.00001929619,0.000014095642,0.9931519,0.00020459936,0.0054924674,0.00011667997,0.000011367666],"about_ca_topic_score_codex":0.021832192,"about_ca_topic_score_gemma":0.009993491,"teacher_disagreement_score":0.021832192,"about_ca_system_score_codex":0.0023617551,"about_ca_system_score_gemma":0.00089781533,"threshold_uncertainty_score":0.04341024},"labels":[],"label_agreement":null},{"id":"W3156234718","doi":"10.3847/1538-4357/abf2b3","title":"Erratum: “The JCMT BISTRO Survey: Magnetic Fields Associated with a Network of Filaments in NGC 1333” (2020, ApJ, 899, 28)","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Manitoba; McMaster University; Queen's University; Western University; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council","keywords":"Physics; Planck; Astrophysics; Magnetic field; Position angle; Paragraph; Astronomy; Galaxy; Quantum mechanics; Law","score_opus":0.010778993002918376,"score_gpt":0.22752211949566425,"score_spread":0.21674312649274588,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3156234718","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0026761584,0.001299452,0.001406571,0.06171658,0.90820044,0.00004490167,0.010628144,0.0013255453,0.012702148],"genre_scores_gemma":[0.05717344,0.006014767,0.011787448,0.1844484,0.337989,0.0004145013,0.045055293,0.0064522936,0.35066485],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9987858,0.00013011522,0.00021611185,0.0002468781,0.0005088992,0.000112268426],"domain_scores_gemma":[0.9935742,0.00095973874,0.0007097412,0.0005630421,0.0037540512,0.00043928478],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011349202,0.0017582205,0.0007237735,0.0024157164,0.003314607,0.002297928,0.0012922186,0.0032204525,0.034892704],"category_scores_gemma":[0.011181225,0.0008154064,0.001023002,0.0019405604,0.0013059642,0.0016853942,0.0014820802,0.0054206615,0.03026317],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039335202,0.000010923961,0.00036852952,0.00006403497,0.000010209593,0.00011760413,0.00003388149,0.000035122117,0.00015921296,0.00036174565,0.9958573,0.002942276],"study_design_scores_gemma":[0.000059348768,0.000041506744,0.009748664,0.00028596364,0.000067706125,0.00040363663,0.00020874236,0.00023067826,0.0008434815,0.0008665756,0.98718286,0.000060893428],"about_ca_topic_score_codex":0.024884786,"about_ca_topic_score_gemma":0.027870113,"teacher_disagreement_score":0.034892704,"about_ca_system_score_codex":0.0022506241,"about_ca_system_score_gemma":0.002936462,"threshold_uncertainty_score":0.11672771},"labels":[],"label_agreement":null},{"id":"W3156265478","doi":"10.3847/1538-4357/ac00b0","title":"Persistent Non-Gaussian Structure in the Image of Sagittarius A* at 86 GHz","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"National Institutes of Natural Sciences; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Japan Society for the Promotion of Science; National Astronomical Observatory of Japan; National Research Foundation; National Research Foundation of Korea; Gordon and Betty Moore Foundation; John Templeton Foundation; Swinburne University of Technology; National Radio Astronomy Observatory; Harvard University; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Scattering; Very-long-baseline interferometry; Supermassive black hole; Sagittarius A*; Galactic Center; Very Long Baseline Array; Wavelength; Interstellar medium; Extrapolation","score_opus":0.00876041671962792,"score_gpt":0.2226574813626152,"score_spread":0.2138970646429873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3156265478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971961,0.000054601922,0.0007114282,0.00010938808,0.000013435505,0.0000029672863,0.0004830849,0.00016741299,0.0012616683],"genre_scores_gemma":[0.9983851,0.000023409702,0.00044375283,0.000027303175,0.000015123436,0.0000026812172,0.00086897,0.000024527777,0.00020908962],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990284,0.000006789436,0.00000398926,0.000025601228,0.00003341903,0.000027391452],"domain_scores_gemma":[0.9996983,0.000019938703,0.00007834293,0.000036913807,0.000060271774,0.000106260726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015281452,0.00015344954,0.00019441325,0.0007111849,0.0002528698,0.00049462775,0.00023163606,0.00022174513,0.0008707635],"category_scores_gemma":[0.0002725488,0.00012930183,0.00024528225,0.00040630612,0.000224714,0.00018029615,0.00036488773,0.00031923188,0.00029385093],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068097946,0.00021754488,0.65668225,0.00007315667,0.000265403,0.00082289096,0.00082001585,0.004692838,0.2984422,0.0011336775,0.006081031,0.030088017],"study_design_scores_gemma":[0.000009473366,0.00003981041,0.99057275,0.000005305478,0.000022157363,0.00017540468,0.00013389668,0.003968948,0.0030332904,0.0001495359,0.0018788374,0.000010538944],"about_ca_topic_score_codex":0.0062058927,"about_ca_topic_score_gemma":0.009583751,"teacher_disagreement_score":0.0062058927,"about_ca_system_score_codex":0.00033511172,"about_ca_system_score_gemma":0.00017617006,"threshold_uncertainty_score":0.012339532},"labels":[],"label_agreement":null},{"id":"W3156846604","doi":"10.3847/1538-4357/abfa23","title":"On the Use of Field RR Lyrae as Galactic Probes. III. The α-element Abundances*","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Istituto Nazionale di Astrofisica; Carnegie Institution of Washington","keywords":"RR Lyrae variable; Metallicity; Galactic halo; Galaxy; Halo; Cepheid variable; Dwarf galaxy; Local Group; Star formation; Globular cluster","score_opus":0.022817704259594614,"score_gpt":0.24127159168751358,"score_spread":0.21845388742791896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3156846604","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99226683,0.0011336759,0.0018290845,0.00003951005,0.000006242652,0.00002452582,0.00075860706,0.000065361965,0.0038761362],"genre_scores_gemma":[0.99540365,0.0002712758,0.0025325771,0.00009815565,0.000024730925,0.000024221128,0.00080090313,0.000018547054,0.0008260287],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994772,0.00018163689,0.000024062645,0.00018464141,0.00007068655,0.000061764076],"domain_scores_gemma":[0.9985713,0.00030234084,0.00035956377,0.00035675304,0.00027093364,0.0001390461],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015536553,0.00042810582,0.00017964818,0.0014196653,0.00025636915,0.0005734679,0.00046061884,0.0002644052,0.0013023608],"category_scores_gemma":[0.0011540888,0.00013596423,0.00016407216,0.00047242572,0.00033539924,0.0005323663,0.0005591249,0.00019525852,0.00096457097],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027906318,0.00004992217,0.9169126,0.00008424033,0.00008139865,0.00010685415,0.00035810695,0.00016772743,0.042604897,0.00025685446,0.00029309426,0.038805224],"study_design_scores_gemma":[0.000009842121,0.00018421792,0.9896219,0.000014453812,0.000034337016,0.00023337528,0.00020420292,0.00027907186,0.0064385105,0.00012323525,0.002850809,0.000006056695],"about_ca_topic_score_codex":0.0021629157,"about_ca_topic_score_gemma":0.003963742,"teacher_disagreement_score":0.0021629157,"about_ca_system_score_codex":0.0002380875,"about_ca_system_score_gemma":0.00008093036,"threshold_uncertainty_score":0.0082166195},"labels":[],"label_agreement":null},{"id":"W3157063504","doi":"10.3847/1538-4357/abf117","title":"The Polarized Image of a Synchrotron-emitting Ring of Gas Orbiting a Black Hole","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Astrophysics Division; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; National Nuclear Security Administration; Toray Science Foundation; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Natural Sciences and Engineering Research Council of Canada; China Scholarship Council; John Templeton Foundation; European Southern Observatory; Ministry of Education, Culture, Sports, Science and Technology; Ministerio de Economía y Competitividad; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Harvard University; Radboud Universiteit; National Research Foundation; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Institutes of Natural Sciences; Government of Canada; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Kavli Foundation; National Astronomical Observatory of Japan; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; Compute Canada; Simons Foundation; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Polarization (electrochemistry); Faraday effect; Rotating black hole; Schwarzschild radius; Black hole (networking); Event horizon; Gravitational lens; Magnetic field; Schwarzschild metric","score_opus":0.009808764792586187,"score_gpt":0.2357997093609194,"score_spread":0.2259909445683332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3157063504","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996505,0.000034890716,0.0013885401,0.000059364527,0.0000065868303,0.0000055959044,0.0000892282,0.000076940865,0.0018338731],"genre_scores_gemma":[0.9993119,0.00001181936,0.00048605565,0.000006937735,0.0000042816687,0.0000015395011,0.000058834867,0.000009795435,0.000108812965],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994946,0.000014411749,0.0000017656675,0.000009049943,0.000008034109,0.000017287735],"domain_scores_gemma":[0.99975306,0.000055091677,0.00005207262,0.000034157227,0.000025700667,0.0000798841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020859709,0.00026864596,0.00028046808,0.00029973662,0.000334734,0.0006554892,0.00046630544,0.0003468784,0.0012178441],"category_scores_gemma":[0.00044317983,0.00019410651,0.00038542354,0.0002603815,0.0005069417,0.00030819935,0.00045241867,0.00030287754,0.00013564271],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022064247,0.0004549935,0.12235421,0.00018446922,0.0005251422,0.00599835,0.00093274424,0.6189698,0.20802681,0.026752736,0.0034975172,0.01009677],"study_design_scores_gemma":[0.000234886,0.00037880402,0.11784331,0.000019238667,0.00008501995,0.0005293071,0.00023001406,0.8615812,0.013664408,0.0044206674,0.0009686689,0.000044478817],"about_ca_topic_score_codex":0.0018153413,"about_ca_topic_score_gemma":0.00075609307,"teacher_disagreement_score":0.0018153413,"about_ca_system_score_codex":0.00037896578,"about_ca_system_score_gemma":0.00015825155,"threshold_uncertainty_score":0.0040740967},"labels":[],"label_agreement":null},{"id":"W3157905823","doi":"10.3847/1538-4357/ac0975","title":"Evidence for Ultra-diffuse Galaxy Formation through Tidal Heating of Normal Dwarfs","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"National Aeronautics and Space Administration","keywords":"Physics; Dwarf galaxy; Astrophysics; Globular cluster; Galaxy; Dwarf spheroidal galaxy; Astronomy; Hubble space telescope; Stars; Interacting galaxy","score_opus":0.032244086216128745,"score_gpt":0.2714376051374788,"score_spread":0.23919351892135005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3157905823","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99853337,0.000073043244,0.00035476542,0.000019645975,0.0000019106392,0.0000025669983,0.000071034265,0.000020401638,0.0009232047],"genre_scores_gemma":[0.9994166,0.000014098324,0.00010065789,0.000011511063,0.0000022180782,9.000234e-7,0.0000937048,0.0000017891696,0.00035846446],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999069,0.0000093944045,0.0000051217608,0.000026155216,0.000020872076,0.000031521184],"domain_scores_gemma":[0.9993993,0.00006213072,0.000103949315,0.00012308244,0.00010139946,0.00021012241],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014299319,0.000111100395,0.00013521255,0.00038601118,0.00021334272,0.0003841104,0.00024798574,0.0001332424,0.0012295007],"category_scores_gemma":[0.00037731582,0.00010619277,0.00011366126,0.00022699249,0.00043977774,0.00015904348,0.00041430228,0.00016180881,0.00023306829],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014484423,0.00003439748,0.9531187,0.000015941156,0.000021829284,0.00022907098,0.00028595724,0.0001630742,0.03842989,0.00037724944,0.00018179564,0.0069972025],"study_design_scores_gemma":[0.0000037314683,0.00006125195,0.99522406,0.0000023676935,0.0000072113435,0.00031484987,0.00013522516,0.0003457816,0.003040598,0.00015599909,0.0007057474,0.0000031236034],"about_ca_topic_score_codex":0.0038773352,"about_ca_topic_score_gemma":0.006763021,"teacher_disagreement_score":0.0038773352,"about_ca_system_score_codex":0.00028939501,"about_ca_system_score_gemma":0.00009078335,"threshold_uncertainty_score":0.007709563},"labels":[],"label_agreement":null},{"id":"W3158086824","doi":"10.3847/1538-4357/ac2b9c","title":"The Irradiation Instability of Protoplanetary Disks","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Starlight; Physics; Instability; Protoplanetary disk; Annulus (botany); Planetesimal; Thermal; Astrophysics; Vortex; Turbulence; Circumstellar disk; Scale height; Planet; Stars; Mechanics; Materials science","score_opus":0.013525307148055981,"score_gpt":0.24733269583872725,"score_spread":0.23380738869067128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3158086824","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99261063,0.0004308604,0.0035927845,0.000077422774,0.000010559246,0.000006628339,0.0000315956,0.00007181472,0.003167735],"genre_scores_gemma":[0.99957806,0.000032307486,0.00017298652,0.000006171975,0.000004517753,0.0000019994445,0.000012475916,0.0000041139947,0.00018749612],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999447,0.000007540239,0.0000030851106,0.000014533511,0.000017437354,0.00001274776],"domain_scores_gemma":[0.99980336,0.000043377375,0.00007818888,0.000016254575,0.00003133325,0.000027499911],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000078787976,0.00021032241,0.00023305697,0.0002631791,0.00040967134,0.00054144126,0.00024328573,0.0002499724,0.00056225475],"category_scores_gemma":[0.0006060361,0.00013613288,0.00017000917,0.00011842752,0.00053919223,0.00029777046,0.0004192335,0.00022328943,0.000112618865],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011414395,0.00012786647,0.1523913,0.00023280088,0.00021361778,0.0022078215,0.0013181253,0.26596108,0.5225518,0.022133455,0.0018675489,0.02985317],"study_design_scores_gemma":[0.00015805782,0.00041305818,0.15614024,0.0000413993,0.00006098212,0.0011575337,0.0005688324,0.7852142,0.038356114,0.014231677,0.003564413,0.00009344855],"about_ca_topic_score_codex":0.0011334362,"about_ca_topic_score_gemma":0.00032193985,"teacher_disagreement_score":0.0011334362,"about_ca_system_score_codex":0.00042361574,"about_ca_system_score_gemma":0.0000878679,"threshold_uncertainty_score":0.0030735135},"labels":[],"label_agreement":null},{"id":"W3158207078","doi":"10.3847/1538-4357/abf7b0","title":"Minimum Orbital Periods of H-rich Bodies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"National Science Foundation","keywords":"White dwarf; Planet; Minimum mass; Range (aeronautics); Orbital inclination; Orbital elements; Orbital period; Brown dwarf; Radial velocity","score_opus":0.011097064423597962,"score_gpt":0.2311028710052839,"score_spread":0.22000580658168595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3158207078","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9892446,0.00033356572,0.0055868383,0.00003973258,0.000007912344,0.0000039032984,0.0006262866,0.00007468419,0.004082465],"genre_scores_gemma":[0.9983498,0.000044772267,0.00093077315,0.000003616629,0.0000043101827,0.0000039066617,0.00047850385,0.000012121038,0.000172328],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99989855,0.000013486674,0.000009251857,0.000026686073,0.000017152914,0.00003478765],"domain_scores_gemma":[0.99933475,0.00033135465,0.00014385916,0.000059346436,0.00006823505,0.00006231387],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031714607,0.00012462912,0.00017331263,0.0007199456,0.00038211647,0.0005009462,0.0002712358,0.00018529782,0.0017266283],"category_scores_gemma":[0.0020954213,0.00012109373,0.00022002637,0.00032497544,0.00018212316,0.00032607248,0.0003464291,0.00016823436,0.00031073342],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014686056,0.00004527564,0.8515513,0.00023703923,0.000120162076,0.00043571834,0.00080543204,0.04167024,0.04134999,0.007849167,0.0021783342,0.052288674],"study_design_scores_gemma":[0.000045609548,0.00014341371,0.9228403,0.00006236429,0.0000470055,0.0009607222,0.00045692915,0.044753473,0.017354224,0.005761294,0.0075430037,0.00003164365],"about_ca_topic_score_codex":0.0010637798,"about_ca_topic_score_gemma":0.0013333948,"teacher_disagreement_score":0.0017266283,"about_ca_system_score_codex":0.000271746,"about_ca_system_score_gemma":0.00013948636,"threshold_uncertainty_score":0.005776167},"labels":[],"label_agreement":null},{"id":"W3158248798","doi":"10.3847/1538-4357/abfcc5","title":"Two-component Magnetic Field along the Line of Sight to the Perseus Molecular Cloud: Contribution of the Foreground Taurus Molecular Cloud","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Herzberg Institute of Astrophysics; University of Calgary; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration","keywords":"Molecular cloud; Physics; Astrophysics; Polarization (electrochemistry); Line-of-sight; Sky; Cloud computing; Position angle; Astronomy; Stars; Optics; Galaxy","score_opus":0.005626451227514449,"score_gpt":0.22795317182763508,"score_spread":0.22232672060012063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3158248798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979462,0.00010900199,0.00031749916,0.000046363588,0.000006252754,0.0000042000793,0.00019462511,0.000042211428,0.0013335609],"genre_scores_gemma":[0.9995303,0.00003438406,0.00011346614,0.000008283911,0.0000115977655,0.0000010018041,0.0001352052,0.0000041324524,0.00016171193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999552,0.000004789011,0.0000014519859,0.000014264741,0.000009629628,0.000014711561],"domain_scores_gemma":[0.99982053,0.00003225808,0.000045392557,0.000013136142,0.000045441157,0.000043239015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007778116,0.0004008269,0.00017056789,0.0007713943,0.0001991123,0.00043506807,0.00020070023,0.00017221914,0.0012426871],"category_scores_gemma":[0.00029628942,0.00012140417,0.00013887283,0.00041533323,0.00014577122,0.00015125972,0.00018651773,0.00012605486,0.00015028541],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042777372,0.00006350769,0.86729014,0.00006603332,0.00011732989,0.0015597974,0.0001564268,0.008613158,0.09553447,0.0007901884,0.00085524115,0.024525994],"study_design_scores_gemma":[0.000027170365,0.000030454272,0.97783625,0.0000093113895,0.000028604612,0.00023460132,0.00010624883,0.017421177,0.0035484673,0.00021712371,0.000534051,0.0000066017756],"about_ca_topic_score_codex":0.011420287,"about_ca_topic_score_gemma":0.0076592825,"teacher_disagreement_score":0.011420287,"about_ca_system_score_codex":0.00036904388,"about_ca_system_score_gemma":0.00018157522,"threshold_uncertainty_score":0.022707641},"labels":[],"label_agreement":null},{"id":"W3158743927","doi":"10.3847/1538-4357/abf653","title":"Erratum: “Secure Mass Measurements from Transit Timing: 10 Kepler Exoplanets between 3 and 8 M <sub>⊕</sub> with Diverse Densities and Incident Fluxes” (2016, ApJ, 820, 39)”","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Université de Montréal","funders":"","keywords":"Exoplanet; Physics; Transit (satellite); Kepler; Planet; Astrobiology; Astronomy; Astrophysics","score_opus":0.027975172624911785,"score_gpt":0.24225110410098546,"score_spread":0.21427593147607368,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3158743927","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.003155912,0.00095642725,0.0013193127,0.0856352,0.85456425,0.000060561615,0.011278273,0.00132795,0.04170212],"genre_scores_gemma":[0.038003374,0.0035157045,0.0076828804,0.091535285,0.092394866,0.00020206337,0.028833658,0.002779681,0.7350525],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99845314,0.00013852525,0.00028453884,0.00025210477,0.0007357894,0.00013584761],"domain_scores_gemma":[0.9930843,0.0013292514,0.00051945384,0.00063049153,0.004014245,0.0004223182],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001633844,0.0015472613,0.0007630541,0.0021761192,0.004720618,0.0030164646,0.0017105719,0.0030025311,0.049702052],"category_scores_gemma":[0.016279409,0.000670509,0.00066111184,0.0014841196,0.0010847745,0.0020462994,0.0018624222,0.004160248,0.039697677],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041209834,0.000012323799,0.0002806157,0.000034056542,0.0000037627494,0.00015378027,0.00003176245,0.000043682954,0.00013171688,0.0005299887,0.9940532,0.004683957],"study_design_scores_gemma":[0.000040562627,0.000037997575,0.0036432773,0.00015620884,0.000028061884,0.0002659448,0.00029574498,0.00030165227,0.0012724858,0.0019435806,0.9919681,0.0000464996],"about_ca_topic_score_codex":0.027822549,"about_ca_topic_score_gemma":0.04693285,"teacher_disagreement_score":0.049702052,"about_ca_system_score_codex":0.0024054446,"about_ca_system_score_gemma":0.0038393054,"threshold_uncertainty_score":0.1662699},"labels":[],"label_agreement":null},{"id":"W3158989835","doi":"10.3847/1538-4357/ac157c","title":"Unexpected Short-period Variability in Dwarf Carbon Stars from the Zwicky Transient Facility","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; University of Oxford; York University; Carnegie Institution for Science; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Astrophysics; Common envelope; Physics; Stars; Light curve; White dwarf; Asymptotic giant branch; Orbital period; Astronomy; Carbon star","score_opus":0.015415661089916412,"score_gpt":0.22892005052239112,"score_spread":0.2135043894324747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3158989835","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939203,0.00001583992,0.000060041475,0.000006067491,6.93983e-7,0.00000170673,0.0002630321,0.00000569612,0.00025487263],"genre_scores_gemma":[0.998782,0.000011310477,0.0001491962,0.0000056600543,0.0000015827931,0.0000027206852,0.000824924,0.0000046911596,0.00021799676],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998634,0.000005508228,0.0000079649735,0.000045447912,0.00003048916,0.00004714163],"domain_scores_gemma":[0.99961793,0.000028097698,0.00016335168,0.00003637583,0.00005828511,0.0000959008],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001369419,0.00012876833,0.00011364239,0.0012817577,0.00039737765,0.00035488012,0.0002439954,0.00014568077,0.00097380683],"category_scores_gemma":[0.00040699518,0.00006957814,0.00009281433,0.00079121214,0.00019960043,0.00022221096,0.00041546824,0.0001062431,0.0002143281],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000062351624,0.000019682062,0.9762793,0.000009213745,0.000014088638,0.00019592892,0.00019013677,0.000083832565,0.0175649,0.00007516244,0.0002503475,0.005254974],"study_design_scores_gemma":[0.000001269498,0.000015069444,0.9981964,0.0000014885723,0.0000031185584,0.00013031416,0.00008009664,0.00011879801,0.001058776,0.000013016294,0.00037997327,0.0000016577804],"about_ca_topic_score_codex":0.012162033,"about_ca_topic_score_gemma":0.032353617,"teacher_disagreement_score":0.012162033,"about_ca_system_score_codex":0.00056172605,"about_ca_system_score_gemma":0.00019064586,"threshold_uncertainty_score":0.024182498},"labels":[],"label_agreement":null},{"id":"W3159076570","doi":"10.3847/1538-4357/abe70d","title":"The Location of Young Pulsar PSR J0837–2454: Galactic Halo or Local Supernova Remnant?","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Science and Technology Facilities Council","keywords":"Pulsar; Physics; Astrophysics; Galactic plane; Supernova remnant; Astronomy; Galaxy; Sky; Population; Supernova; Surface brightness; Milky Way","score_opus":0.01501278230178936,"score_gpt":0.3114623199088684,"score_spread":0.29644953760707904,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3159076570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99788445,0.00048110864,0.00013058765,0.00008060977,0.000011167627,0.0000027981523,0.00013322828,0.000019559444,0.0012564176],"genre_scores_gemma":[0.99955577,0.00009373814,0.00006285274,0.000012602598,0.000014681303,6.56927e-7,0.00009710409,0.0000023600785,0.00016027357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994206,0.0000050901817,0.000004898958,0.000015522513,0.000012931222,0.000019609928],"domain_scores_gemma":[0.9996717,0.000022178692,0.00013837143,0.000026283024,0.000041857038,0.000099693905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019195954,0.00014869422,0.00021232177,0.00092610554,0.0003750503,0.0006241493,0.00029654373,0.00023156738,0.0023308885],"category_scores_gemma":[0.0004573447,0.00008821421,0.0001480543,0.00048151956,0.00046029428,0.00029844203,0.00045182588,0.0001592239,0.00060700206],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014854112,0.000022085638,0.9802356,0.000022720355,0.00003885484,0.003669627,0.0001801863,0.00011376407,0.008123218,0.0002567694,0.00039832608,0.006790313],"study_design_scores_gemma":[0.000009153932,0.0001010109,0.9906211,0.000019245936,0.000041696258,0.004494006,0.00044383426,0.00037309635,0.0019740015,0.00018098907,0.0017305427,0.000011328322],"about_ca_topic_score_codex":0.0071545937,"about_ca_topic_score_gemma":0.006217485,"teacher_disagreement_score":0.0071545937,"about_ca_system_score_codex":0.00038691008,"about_ca_system_score_gemma":0.0001714471,"threshold_uncertainty_score":0.0142259},"labels":[],"label_agreement":null},{"id":"W3159152270","doi":"10.3847/1538-4357/abf4fd","title":"870 μm Dust Continuum of the Youngest Protostars in Ophiuchus","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"National Institutes of Natural Sciences; National Astronomical Observatory of Japan; Associated Universities; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Ophiuchus; Physics; Astrophysics; Protostar; Astronomy; Star formation; Molecular cloud; Stellar mass; RADIUS; Stars","score_opus":0.009562445261136806,"score_gpt":0.23129866422560938,"score_spread":0.22173621896447257,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3159152270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907047,0.00006395903,0.00009491438,0.0000073352858,7.467505e-7,0.0000019804545,0.0002804146,0.000019510031,0.0004608099],"genre_scores_gemma":[0.99899036,0.000038843053,0.00020515431,0.000013243061,0.0000036994181,0.0000032704402,0.0004939871,0.0000048259767,0.00024667164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999058,0.000007323678,0.000005963104,0.000029708826,0.000023796567,0.000027316146],"domain_scores_gemma":[0.9997874,0.000022808366,0.000057679885,0.000019521834,0.000036199774,0.00007642786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001353507,0.00013737402,0.00019995742,0.0012049386,0.00039209842,0.00049497915,0.00016115779,0.00013991143,0.00095939764],"category_scores_gemma":[0.00023754421,0.00012620051,0.00011285279,0.00061057083,0.00016549442,0.00018148126,0.00048491152,0.00010114527,0.00032076245],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010507679,0.000029092302,0.9669399,0.000019393685,0.00002575521,0.00012049445,0.00030435759,0.00017983987,0.023785831,0.00007056291,0.00026912027,0.008150634],"study_design_scores_gemma":[0.0000013910193,0.000009110619,0.99900097,0.0000015688664,0.000004095301,0.0000376742,0.00006495925,0.00010752645,0.0005056448,0.000014685823,0.0002515294,9.810442e-7],"about_ca_topic_score_codex":0.0069287196,"about_ca_topic_score_gemma":0.011508854,"teacher_disagreement_score":0.0069287196,"about_ca_system_score_codex":0.00028077606,"about_ca_system_score_gemma":0.00014356304,"threshold_uncertainty_score":0.013776779},"labels":[],"label_agreement":null},{"id":"W3159459364","doi":"10.3847/1538-4357/abfc58","title":"The MAVERIC Survey: Dynamical Origin of Radio Sources in Galactic Globular Clusters","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Australian Research Council; Natural Sciences and Engineering Research Council of Canada; David and Lucile Packard Foundation; National Science Foundation","keywords":"Globular cluster; Neutron star; Millisecond pulsar; Star cluster; RADIUS; Luminosity; Cluster (spacecraft); Pulsar; White dwarf","score_opus":0.013419192839145331,"score_gpt":0.23931846830295908,"score_spread":0.22589927546381375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3159459364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992219,0.00008383277,0.00012265498,0.000015331587,8.8518277e-7,0.000001927349,0.00022513859,0.000006259565,0.00032213493],"genre_scores_gemma":[0.9993279,0.000035576202,0.00010717909,0.00000868759,0.0000026186815,0.0000017907178,0.00040420893,0.0000035154233,0.000108566346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99949646,0.00015684386,0.000028296812,0.00015759276,0.00007816995,0.00008268764],"domain_scores_gemma":[0.9968766,0.0009469679,0.0008826249,0.00042696926,0.00041754002,0.00044923442],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087328575,0.00018839643,0.0002048498,0.0015049909,0.00032153187,0.0007808681,0.00042393568,0.00022768698,0.0008274769],"category_scores_gemma":[0.0035386276,0.000111646055,0.0001871166,0.0011629659,0.00032017156,0.00023187383,0.0005714311,0.00016395486,0.00017052235],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00001816851,0.0000021878056,0.99824154,0.0000019462627,0.000015770749,0.000015314734,0.000060166614,0.00016363329,0.00047514192,0.000057889818,0.000034196128,0.0009140124],"study_design_scores_gemma":[0.000001385723,0.000012448063,0.9991134,0.000002263595,0.000006879169,0.00003418495,0.00007477619,0.00040897648,0.00012426163,0.000017895543,0.0002019196,0.0000015842367],"about_ca_topic_score_codex":0.02234294,"about_ca_topic_score_gemma":0.03893664,"teacher_disagreement_score":0.02234294,"about_ca_system_score_codex":0.00044087516,"about_ca_system_score_gemma":0.0003120477,"threshold_uncertainty_score":0.044425786},"labels":[],"label_agreement":null},{"id":"W3159488228","doi":"10.3847/1538-4357/abfc52","title":"WALLABY Pilot Survey: The Diversity of Ram Pressure Stripping of the Galactic H i Gas in the Hydra Cluster","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Ministry of Science and ICT, South Korea; Government of Western Australia; National Central University; National Research Foundation of Korea; Instituto de Astrofísica de Andalucía; Queen's University; Smithsonian Institution; National Natural Science Foundation of China; National Research Foundation; Space Telescope Science Institute; Science and Industry Endowment Fund; Australian Government; Queen's University Belfast; Ministerio de Ciencia, Innovación y Universidades; Gordon and Betty Moore Foundation; Eötvös Loránd Tudományegyetem; European Commission; Los Alamos National Laboratory; Johns Hopkins University; Peking University; Commonwealth Scientific and Industrial Research Organisation; National Aeronautics and Space Administration; Durham University; National Science Foundation","keywords":"Galaxy; Ram pressure; Stripping (fiber); Cluster (spacecraft); Lernaean Hydra; Galaxy cluster; Star formation","score_opus":0.015099682130441728,"score_gpt":0.21423815875053512,"score_spread":0.1991384766200934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3159488228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998295,0.00004455085,0.000054590153,0.000024756066,0.0000013252389,0.0000062245435,0.00085749134,0.000017030861,0.0006990772],"genre_scores_gemma":[0.99621034,0.000069410846,0.00023822476,0.0000340113,0.0000057937355,0.000018686129,0.0026939842,0.000017483706,0.00071207166],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973327,0.00003822245,0.000013115083,0.00008353226,0.000049610593,0.000082306724],"domain_scores_gemma":[0.99933976,0.0000665083,0.00013966535,0.00012667956,0.00008903513,0.000238384],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034507387,0.00019993662,0.00027479636,0.0009205469,0.00051095145,0.00057131844,0.00034691757,0.00016139845,0.0017699803],"category_scores_gemma":[0.00082972756,0.00020404355,0.00016630164,0.00084546977,0.00044695716,0.00043377245,0.0015287057,0.00017668027,0.0004612355],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003762656,0.00003558172,0.9744974,0.000034314322,0.000074503405,0.0003030336,0.0015463161,0.00016621729,0.011018291,0.00015621506,0.001888868,0.009903003],"study_design_scores_gemma":[0.0000037201544,0.000015330654,0.9987305,0.0000026170712,0.000004800145,0.00004337506,0.00025824137,0.000068457826,0.00026860612,0.000012523342,0.00058846665,0.000003343801],"about_ca_topic_score_codex":0.03147078,"about_ca_topic_score_gemma":0.05262342,"teacher_disagreement_score":0.03147078,"about_ca_system_score_codex":0.00030680388,"about_ca_system_score_gemma":0.00029099835,"threshold_uncertainty_score":0.06257516},"labels":[],"label_agreement":null},{"id":"W3160003518","doi":"10.3847/1538-4357/ac2dfc","title":"Comparative Study of Electric Currents and Energetic Particle Fluxes in a Solar Flare and Earth Magnetospheric Substorm","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Natural Resources Canada","funders":"Air Force Office of Scientific Research; Japan Aerospace Exploration Agency; UC Berkeley College of Chemistry; Budget Division; Russian Science Foundation; National Aeronautics and Space Administration; Natural Resources Canada; Canadian Space Agency; National Science Foundation","keywords":"Substorm; Physics; Magnetic reconnection; Solar flare; Flare; Interplanetary magnetic field; Geophysics; Astrophysics; Particle acceleration; Ionosphere; Photosphere; Plasma; Magnetosphere; Solar wind; Computational physics; Magnetic field","score_opus":0.009063773189611487,"score_gpt":0.2360629307013501,"score_spread":0.2269991575117386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3160003518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99838483,0.000068235626,0.00019663642,0.0000068380928,0.0000021555813,0.0000059328795,0.00079725264,0.000018032857,0.000520113],"genre_scores_gemma":[0.9971003,0.000043372296,0.00019426292,0.0000044749954,0.000005795798,0.000007208064,0.0025158103,0.000005990073,0.00012271105],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998783,0.0000138377245,0.000011985562,0.000035659334,0.000029544277,0.00003054905],"domain_scores_gemma":[0.9992501,0.0002295669,0.0002075937,0.00006376047,0.00015303248,0.00009578939],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023515579,0.00019537583,0.00034228512,0.0015370533,0.0002501078,0.000514868,0.00020452445,0.00030009318,0.00085633266],"category_scores_gemma":[0.00079939736,0.000110066685,0.0002505066,0.0010951431,0.00020144161,0.00039340375,0.0003249432,0.00015260353,0.0001570328],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052129355,0.0001460558,0.91352177,0.00009388543,0.00024507448,0.00056412787,0.0006343722,0.0030408616,0.06158728,0.00028209458,0.00056727143,0.018795911],"study_design_scores_gemma":[0.0000035445685,0.000036119134,0.9972045,0.000003379652,0.000012406425,0.00009224127,0.00008047928,0.0013689982,0.0008916975,0.00002837574,0.0002735788,0.00000471855],"about_ca_topic_score_codex":0.005268391,"about_ca_topic_score_gemma":0.004445815,"teacher_disagreement_score":0.005268391,"about_ca_system_score_codex":0.00024387304,"about_ca_system_score_gemma":0.00008916846,"threshold_uncertainty_score":0.010475457},"labels":[],"label_agreement":null},{"id":"W3160448744","doi":"10.3847/1538-4357/abeb71","title":"Searches after Gravitational Waves Using ARizona Observatories (SAGUARO): Observations and Analysis from Advanced LIGO/Virgo's Third Observing Run","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"LIGO; Gravitational wave; Physics; Telescope; Astronomy; Astrophysics","score_opus":0.033429228338518885,"score_gpt":0.3147486158570434,"score_spread":0.2813193875185245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3160448744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9899474,0.00009130359,0.0010686807,0.00004506057,0.0000048345914,0.000024629751,0.006815754,0.00024993825,0.0017524156],"genre_scores_gemma":[0.968286,0.00009342458,0.0031242152,0.000047069392,0.00001555868,0.000026584927,0.027350634,0.00010493346,0.00095146283],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979395,0.000023069388,0.000012703921,0.000047439615,0.00006727428,0.000055610246],"domain_scores_gemma":[0.99898726,0.00015317749,0.0002946298,0.00016140427,0.00015197763,0.00025160392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038269447,0.00023503765,0.00023063598,0.0014600132,0.00028986915,0.0006005493,0.0002877791,0.00015886342,0.001187238],"category_scores_gemma":[0.00081241503,0.00013292489,0.00040626724,0.0014759284,0.00017706833,0.00021094801,0.00068473426,0.00029299353,0.0003115269],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029589102,0.00004908619,0.9657192,0.00005078529,0.0001654021,0.00028695838,0.0002380355,0.001529993,0.008937943,0.0002663409,0.004029949,0.018430367],"study_design_scores_gemma":[0.0000067186543,0.000020161202,0.9957262,0.0000053993112,0.00003343124,0.00005061652,0.000075396245,0.0017626495,0.00083928904,0.00003534337,0.0014371583,0.000007542008],"about_ca_topic_score_codex":0.024235124,"about_ca_topic_score_gemma":0.05552752,"teacher_disagreement_score":0.024235124,"about_ca_system_score_codex":0.00032480567,"about_ca_system_score_gemma":0.00034246087,"threshold_uncertainty_score":0.04818815},"labels":[],"label_agreement":null},{"id":"W3161054069","doi":"10.3847/1538-4357/abffcc","title":"Predicting the Spectrum of UGC 2885, Rubin’s Galaxy with Machine Learning","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Galaxy; Physics; Astrophysics; Spectral line; Active galactic nucleus; Galaxy merger; Universe; Emission spectrum; Galaxy formation and evolution; Astronomy","score_opus":0.006550764541595405,"score_gpt":0.20045657588191274,"score_spread":0.19390581134031734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161054069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9934993,0.00006275542,0.005136102,0.00006924097,0.000003777936,0.000005142939,0.00015082251,0.0002395983,0.00083335006],"genre_scores_gemma":[0.9965598,0.000008593957,0.0029662503,0.000009284382,0.0000026914267,0.0000012758486,0.00031747107,0.000009525134,0.00012510354],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998771,0.000033042103,0.0000036701822,0.00003946021,0.000025201265,0.000021517439],"domain_scores_gemma":[0.9995413,0.0001378044,0.00007986429,0.00008498283,0.00007119187,0.00008500893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053224474,0.00027825107,0.00017999126,0.0007435094,0.0001505054,0.00057012687,0.00039517827,0.0003698353,0.0005571978],"category_scores_gemma":[0.0015595239,0.000110354544,0.0003036104,0.00032159808,0.00018404746,0.00031862498,0.00027241601,0.0002476762,0.00029360421],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045921665,0.00017157283,0.80471814,0.000050393468,0.00018029237,0.0001563825,0.00011873547,0.10635592,0.018429337,0.001275867,0.002032553,0.066051595],"study_design_scores_gemma":[0.000028234479,0.000083192404,0.22587489,0.000009121058,0.000032722503,0.000061853185,0.0000930717,0.7633416,0.008648943,0.0010403609,0.00077075866,0.000015303709],"about_ca_topic_score_codex":0.0052764816,"about_ca_topic_score_gemma":0.0047654854,"teacher_disagreement_score":0.0052764816,"about_ca_system_score_codex":0.00048148265,"about_ca_system_score_gemma":0.0001367964,"threshold_uncertainty_score":0.01049149},"labels":[],"label_agreement":null},{"id":"W3161228155","doi":"10.3847/1538-4357/abffcf","title":"Fresh Insights on the Kinematics of M49's Globular Cluster System with MMT/Hectospec Spectroscopy","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Globular cluster; Virgo Cluster; Galaxy; Halo; Velocity dispersion; Kinematics; Stellar kinematics; Dwarf galaxy; Star cluster","score_opus":0.005766888179571393,"score_gpt":0.19515112413331048,"score_spread":0.1893842359537391,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161228155","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931625,0.00009929133,0.00082188286,0.0000658407,0.00000440963,0.000014698193,0.0024282627,0.00006813385,0.003335014],"genre_scores_gemma":[0.99402374,0.000053243097,0.00236765,0.00007378675,0.000017322584,0.000010649147,0.0029497172,0.000026135973,0.00047795696],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983275,0.000014889854,0.0000072867083,0.000052669533,0.00004951154,0.00004297164],"domain_scores_gemma":[0.99954116,0.00003161555,0.00014465746,0.000099855766,0.000096340395,0.000086312786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003543735,0.00020589195,0.00014687204,0.0015702089,0.00049814134,0.00055324537,0.00036422806,0.0002864444,0.0012715457],"category_scores_gemma":[0.00056431856,0.00011650467,0.00021964134,0.0009757413,0.00022731327,0.0003541636,0.0007643324,0.00022295842,0.000631715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048722013,0.000026913907,0.94830626,0.000015739293,0.000037101647,0.0002431969,0.0003852691,0.00041547063,0.040173333,0.00031846823,0.0012093751,0.008820163],"study_design_scores_gemma":[0.0000013538339,0.000009621572,0.9979017,0.0000037827028,0.000005669624,0.000075650445,0.00010681872,0.00035575795,0.0007070856,0.000041929823,0.00078711566,0.0000035435912],"about_ca_topic_score_codex":0.010779014,"about_ca_topic_score_gemma":0.02511413,"teacher_disagreement_score":0.010779014,"about_ca_system_score_codex":0.00040305423,"about_ca_system_score_gemma":0.00013360767,"threshold_uncertainty_score":0},"labels":[],"label_agreement":null},{"id":"W3161297225","doi":"10.3847/1538-4357/abf7c2","title":"Erratum: “Mapping Metallicity Variations across Nearby Galaxy Disks” (2019, ApJ, 887, 80)","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Deutsche Forschungsgemeinschaft","keywords":"Metallicity; Physics; Table (database); Galaxy; Astrophysics; Astronomy; Computer science; Data mining","score_opus":0.016962299460999173,"score_gpt":0.25390225670989663,"score_spread":0.23693995724889746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161297225","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00051162136,0.000985681,0.00045734394,0.05720771,0.90632176,0.000044694578,0.0072583593,0.00082460983,0.026388258],"genre_scores_gemma":[0.0063763466,0.0028279435,0.002682051,0.083338454,0.15330568,0.00014234222,0.012390061,0.002085505,0.7368516],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988462,0.00011847841,0.00017179032,0.00017086585,0.00059065234,0.00010207986],"domain_scores_gemma":[0.99205494,0.001279657,0.0004184287,0.00050232926,0.00509483,0.0006498374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014361113,0.0018099603,0.0010699241,0.0038708944,0.004680019,0.0042319954,0.0016852564,0.003801165,0.117292665],"category_scores_gemma":[0.014305583,0.0006717738,0.0010013522,0.0021445225,0.0010938221,0.002413898,0.0017237983,0.004367204,0.093255915],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000012081493,0.0000034956543,0.00005368756,0.000015972351,0.0000015906749,0.000042852877,0.000004678407,0.000009675882,0.000032632975,0.00010370906,0.99815696,0.0015627459],"study_design_scores_gemma":[0.000028552393,0.000022471297,0.0021522406,0.00015005052,0.000015625305,0.00016490514,0.00010344824,0.000110211055,0.00026510036,0.000845825,0.9961139,0.0000276223],"about_ca_topic_score_codex":0.039156597,"about_ca_topic_score_gemma":0.06802622,"teacher_disagreement_score":0.117292665,"about_ca_system_score_codex":0.0024640851,"about_ca_system_score_gemma":0.0035602145,"threshold_uncertainty_score":0.3923831},"labels":[],"label_agreement":null},{"id":"W3161312350","doi":"10.3847/1538-4357/ac3252","title":"The 3D Kinematics of the Orion Nebula Cluster: NIRSPEC-AO Radial Velocities of the Core Population","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; NASA Exoplanet Science Institute; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Universidad Nacional Autónoma de México; Space Telescope Science Institute; W. M. Keck Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; University of California, San Diego; Yale University; National Science Foundation","keywords":"Physics; Algorithm; Computer science","score_opus":0.010602275402403332,"score_gpt":0.22938928545118975,"score_spread":0.21878701004878642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161312350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948973,0.00006367008,0.0011271716,0.000022417773,0.0000037781792,0.000005900799,0.0014387022,0.00009417816,0.0023467273],"genre_scores_gemma":[0.993995,0.00003913324,0.0022426085,0.000007586252,0.000005497709,0.000005552444,0.0025921152,0.000048644913,0.0010638349],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999167,0.00000707149,0.0000022002978,0.000034156434,0.000023954686,0.000016034128],"domain_scores_gemma":[0.99975663,0.000026243877,0.000059310823,0.00003173136,0.00007378142,0.00005225304],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024153336,0.00020188771,0.00012538867,0.0010997839,0.00019337812,0.0004907923,0.00021376174,0.0001301766,0.0014429415],"category_scores_gemma":[0.00048193673,0.00014984369,0.00019777779,0.0006278669,0.000144271,0.00020574183,0.00037952454,0.00013702772,0.0005675401],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017157786,0.000045679037,0.9210058,0.000020920688,0.00007596633,0.0001123258,0.00047972132,0.011765549,0.035342928,0.00076290034,0.0019790486,0.028237782],"study_design_scores_gemma":[0.0000032015992,0.0000104037945,0.98953724,0.00000363892,0.000010181746,0.000044245426,0.000052620213,0.0074851057,0.0016210517,0.00010607762,0.00111501,0.0000112450225],"about_ca_topic_score_codex":0.023836276,"about_ca_topic_score_gemma":0.030192247,"teacher_disagreement_score":0.023836276,"about_ca_system_score_codex":0.0005055127,"about_ca_system_score_gemma":0.00024443245,"threshold_uncertainty_score":0.04739511},"labels":[],"label_agreement":null},{"id":"W3161932522","doi":"10.3847/1538-4357/ac0444","title":"Evaluating Rotation Periods of M Dwarfs across the Ages","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"","keywords":"Photometry (optics); Rotation (mathematics); Rotation period; Physics; Pleiades; Astrophysics; Light curve; Stars; Artificial intelligence; Computer science","score_opus":0.029128981100723945,"score_gpt":0.32178363178351954,"score_spread":0.2926546506827956,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3161932522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951186,0.00016518985,0.0017331952,0.000017292103,0.000006677823,0.0000069986986,0.0008559388,0.0001261423,0.001969879],"genre_scores_gemma":[0.9973219,0.00004632844,0.0009207077,0.0000066741113,0.0000061161154,0.000003788633,0.0012530147,0.000038308237,0.0004032837],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999696,0.000054082306,0.00002091258,0.000105656305,0.00006740184,0.000055942815],"domain_scores_gemma":[0.99838805,0.00037850646,0.0004937952,0.00016727186,0.00031569577,0.00025657832],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089138915,0.00029433012,0.00023323145,0.0016299216,0.00030979072,0.0004958159,0.00016955264,0.00017638132,0.0011492743],"category_scores_gemma":[0.0030370727,0.00010793052,0.00022628265,0.0007332723,0.0002268205,0.00039563156,0.00040618802,0.00013298435,0.0008160298],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023015241,0.000012246061,0.97399634,0.000018228384,0.000040360374,0.00004715281,0.00023044476,0.0028760962,0.004403758,0.00016726197,0.0005543984,0.017423531],"study_design_scores_gemma":[0.000004975286,0.00006604061,0.9895225,0.0000061791025,0.000016723337,0.00010900608,0.0002740376,0.004784294,0.003043823,0.00022044501,0.0019424811,0.00000953157],"about_ca_topic_score_codex":0.005565635,"about_ca_topic_score_gemma":0.006788492,"teacher_disagreement_score":0.005565635,"about_ca_system_score_codex":0.00043634645,"about_ca_system_score_gemma":0.0001626576,"threshold_uncertainty_score":0.011066496},"labels":[],"label_agreement":null},{"id":"W3162310438","doi":"10.3847/1538-4357/abff5c","title":"A Deep Polarimetric Study of the Asymmetrical Debris Disk HD 106906","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Debris disk; Planet; Debris; Brightness; Planetary system; Flux (metallurgy); Surface brightness; Planetesimal; Stars","score_opus":0.011399925974307612,"score_gpt":0.23008466990402268,"score_spread":0.21868474392971507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3162310438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99762565,0.00005893888,0.0003121154,0.000016977554,0.000004134155,0.000004816246,0.0006179502,0.00001811529,0.0013412086],"genre_scores_gemma":[0.99810946,0.000037269314,0.0005385836,0.000017424216,0.0000064194446,0.000001489553,0.001023318,0.000007148021,0.0002589313],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999397,0.0000054653315,0.000002929256,0.000018197614,0.000016220041,0.000017480388],"domain_scores_gemma":[0.9998776,0.000016873959,0.000031436262,0.000016497292,0.000027362876,0.000030166293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009251381,0.0001938594,0.00016152007,0.00073492853,0.00021788695,0.00028321156,0.000120113684,0.00017672947,0.0007909562],"category_scores_gemma":[0.00015540855,0.00012801807,0.00013219517,0.0005356919,0.00018376793,0.00021494244,0.00043579048,0.0002075573,0.00032318034],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005177326,0.00019681781,0.27933568,0.000070169524,0.00007030597,0.0009872768,0.0006579818,0.0015665197,0.6925185,0.00028556306,0.00087479723,0.022918688],"study_design_scores_gemma":[0.000011589816,0.000073620016,0.98473626,0.0000042186466,0.000015594373,0.00062721537,0.0002204965,0.0012367925,0.011978913,0.000054529362,0.0010321068,0.000008679361],"about_ca_topic_score_codex":0.002120858,"about_ca_topic_score_gemma":0.0036115614,"teacher_disagreement_score":0.002120858,"about_ca_system_score_codex":0.00013070212,"about_ca_system_score_gemma":0.00004889265,"threshold_uncertainty_score":0.0042170286},"labels":[],"label_agreement":null},{"id":"W3162486600","doi":"10.3847/1538-4357/abfe14","title":"Longitudinally Resolved Spectral Retrieval (ReSpect) of WASP-43b","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Exoplanet; Spectral line; James Webb Space Telescope; Stellar classification; Spectral shape analysis; Phase retrieval; Range (aeronautics); Planet","score_opus":0.01454430032325444,"score_gpt":0.23603937030255306,"score_spread":0.22149506997929863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3162486600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9789488,0.00007859077,0.016456993,0.00012982228,0.00002293961,0.000025268879,0.0011455639,0.0013629035,0.0018291174],"genre_scores_gemma":[0.98854595,0.000023660521,0.009984857,0.00002019781,0.0000051542124,0.000007428552,0.001066268,0.00009504603,0.00025131175],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999019,0.000010711027,0.000005019033,0.000029538072,0.000032021377,0.000020734742],"domain_scores_gemma":[0.99981505,0.00003449499,0.000027909546,0.000041903662,0.000050046623,0.000030671792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029779715,0.00033109522,0.00024481822,0.00041684124,0.00034027005,0.00055302447,0.00048443076,0.00044612054,0.0016509396],"category_scores_gemma":[0.0010638761,0.00024561712,0.0006384687,0.0005300824,0.0002623466,0.00070358213,0.00040669017,0.00051218295,0.00040884735],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073109765,0.00040605463,0.1100992,0.00018880845,0.00027999002,0.00040495285,0.00036113316,0.67171866,0.1453581,0.002427024,0.002769571,0.06525547],"study_design_scores_gemma":[0.000069009206,0.00006240095,0.03127613,0.000008596589,0.000023581528,0.0000524656,0.0000619957,0.95148385,0.015336921,0.0005687089,0.001031428,0.000024830546],"about_ca_topic_score_codex":0.015217306,"about_ca_topic_score_gemma":0.011862927,"teacher_disagreement_score":0.015217306,"about_ca_system_score_codex":0.00047855146,"about_ca_system_score_gemma":0.0006399174,"threshold_uncertainty_score":0.030257463},"labels":[],"label_agreement":null},{"id":"W3162586086","doi":"10.3847/1538-4357/abec74","title":"Extended X-Ray Emission Associated with the Radio Lobes and the Environments of 60 Radio Galaxies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Radio galaxy; Redshift; X-shaped radio galaxy; Intracluster medium; Galaxy; Astronomy; Galaxy cluster; Optics","score_opus":0.004625720431917741,"score_gpt":0.18770758912250404,"score_spread":0.1830818686905863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3162586086","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99970466,0.0000594788,0.00006503006,0.000002041187,2.4739958e-7,0.0000010438067,0.00006288873,0.0000030398169,0.000101644546],"genre_scores_gemma":[0.99951565,0.00004856545,0.00009935955,0.0000033258514,0.0000023806674,0.0000012172277,0.00026224132,0.0000018705828,0.000065377644],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998436,0.000018115523,0.000015595811,0.00004121138,0.000036003046,0.00004544021],"domain_scores_gemma":[0.9989712,0.00020108918,0.0004729494,0.00009399243,0.0001095617,0.00015120667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027552777,0.0002208631,0.00026910123,0.0012617542,0.00016818735,0.000605492,0.0002172093,0.00014314298,0.00064385374],"category_scores_gemma":[0.0008428808,0.00015528606,0.00025735635,0.0007283571,0.00032609675,0.00020842909,0.0005689312,0.00014079794,0.00019325444],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000066047396,0.000015722544,0.9874955,0.000012697787,0.00003481834,0.000113778544,0.00019165472,0.00017609145,0.008222863,0.000047732254,0.000022377015,0.0036007236],"study_design_scores_gemma":[0.0000017349893,0.000020575575,0.9989267,0.0000012755621,0.000010886954,0.0001636374,0.00006326455,0.0001488521,0.00054707774,0.000017298455,0.00009696203,0.0000018233617],"about_ca_topic_score_codex":0.0022543364,"about_ca_topic_score_gemma":0.0027392167,"teacher_disagreement_score":0.0022543364,"about_ca_system_score_codex":0.00017239607,"about_ca_system_score_gemma":0.000104552455,"threshold_uncertainty_score":0.0044823885},"labels":[],"label_agreement":null},{"id":"W3162609793","doi":"10.3847/1538-4357/aca591","title":"4-OGC: Catalog of Gravitational Waves from Compact Binary Mergers","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":230,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; Agencia Estatal de Investigación; National Science Foundation","keywords":"Physics; Algorithm; Database; Computer science","score_opus":0.019232932359056407,"score_gpt":0.325745838004569,"score_spread":0.3065129056455126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3162609793","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2064956,0.0026810823,0.0051503936,0.0005111587,0.00020335436,0.00077067694,0.7325165,0.004493712,0.04717755],"genre_scores_gemma":[0.06996108,0.0008299815,0.0064619984,0.00023675642,0.00017804423,0.00034475562,0.9151422,0.0005149979,0.0063301865],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99903584,0.00007250008,0.000112337664,0.00014932308,0.0004352229,0.00019485601],"domain_scores_gemma":[0.9956281,0.00034005562,0.0011128216,0.0008727913,0.0013294372,0.0007168213],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009503319,0.0008448082,0.0005906316,0.012771375,0.0009186871,0.0019268135,0.0008285338,0.0005363605,0.009624467],"category_scores_gemma":[0.0039362204,0.00032159442,0.0004902579,0.010440124,0.00030903317,0.0012011325,0.0021079106,0.00060535205,0.006390963],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006887575,0.00014957291,0.33445618,0.00063352124,0.00014567006,0.00048061155,0.0006594329,0.0014800165,0.0049257283,0.0070436206,0.500751,0.14858589],"study_design_scores_gemma":[0.00013277955,0.000062213534,0.43664873,0.00020920625,0.00009011722,0.00041915095,0.00030936714,0.00294714,0.0025561377,0.0023007444,0.5542492,0.000075233016],"about_ca_topic_score_codex":0.030004296,"about_ca_topic_score_gemma":0.024698947,"teacher_disagreement_score":0.030004296,"about_ca_system_score_codex":0.0012004675,"about_ca_system_score_gemma":0.0019830454,"threshold_uncertainty_score":0.059659302},"labels":[],"label_agreement":null},{"id":"W3163482491","doi":"10.3847/1538-4357/ac1589","title":"Kinematics of Crab Giant Pulses","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Queen's University; Perimeter Institute; University of Toronto; Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research","funders":"","keywords":"Physics; Pulsar; Astrophysics; Lorentz factor; Crab Nebula; Crab Pulsar; Scattering; Brightness; Plasma; Doppler effect; Pulse (music); Optics; Astronomy","score_opus":0.01868764641108579,"score_gpt":0.3295504524661029,"score_spread":0.31086280605501715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3163482491","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9772953,0.00044894434,0.0054112654,0.00010230435,0.000021545811,0.000012847422,0.00035929008,0.0001406147,0.016207848],"genre_scores_gemma":[0.9969674,0.00007750717,0.0010777442,0.000018941,0.0000058745522,0.000005106694,0.00018525019,0.00003558157,0.0016266463],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999567,0.0000039125616,0.0000012887944,0.000013191365,0.000012653642,0.000012171918],"domain_scores_gemma":[0.9998211,0.00005102983,0.00004254145,0.00001645124,0.000037242367,0.000031641477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000070933515,0.00014925346,0.00011407517,0.0005871777,0.0002376056,0.00042139814,0.00014258201,0.00027268523,0.0026324138],"category_scores_gemma":[0.00042082046,0.000139449,0.000088955465,0.00036329523,0.00015572348,0.00017105111,0.00040712266,0.00028369587,0.0006182283],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058072706,0.00009895033,0.3111493,0.00028525825,0.00011142677,0.003387175,0.0022830553,0.016808946,0.51619947,0.018669961,0.005143373,0.1252824],"study_design_scores_gemma":[0.000030240615,0.00025350988,0.9051459,0.00007907887,0.00003615305,0.0029957748,0.0010824732,0.02095864,0.04495101,0.00805094,0.016355937,0.00006032032],"about_ca_topic_score_codex":0.0012567635,"about_ca_topic_score_gemma":0.0011454544,"teacher_disagreement_score":0.0026324138,"about_ca_system_score_codex":0.00020977345,"about_ca_system_score_gemma":0.000103261125,"threshold_uncertainty_score":0.008806288},"labels":[],"label_agreement":null},{"id":"W3163849276","doi":"10.3847/1538-4357/ac2159","title":"AGN STORM 2. I. First results: A Change in the Weather of Mrk 817","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Instituto de Astrofísica de Andalucía; People's Government of Yunnan Province; National Natural Science Foundation of China; Liverpool John Moores University; Chinese Academy of Sciences; Grantová Agentura České Republiky; University of Leicester; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Alexander von Humboldt-Stiftung; National Aeronautics and Space Administration; Youth Innovation Promotion Association; Space Telescope Science Institute; University of California, Irvine; Youth Innovation Promotion Association of the Chinese Academy of Sciences; National Science Foundation","keywords":"Astrophysics; Physics; Galaxy; Accretion disc; Active galactic nucleus; Emission spectrum; Reverberation mapping; Accretion (finance); Quasar; Astronomy; Ionization; Wavelength; Line (geometry); Spectral line; Optics","score_opus":0.03428720664421834,"score_gpt":0.2635053028922976,"score_spread":0.2292180962480793,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3163849276","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924056,0.000091637485,0.00032007144,0.00022436726,0.00006312999,0.00002723917,0.003052358,0.00015842312,0.0036573007],"genre_scores_gemma":[0.99204797,0.00005436756,0.00040220335,0.00013872601,0.00009623751,0.00002090935,0.006001904,0.000050014005,0.0011876882],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99960583,0.000029644647,0.000019365232,0.00009886102,0.00013818283,0.00010801657],"domain_scores_gemma":[0.9989899,0.0001404672,0.000181359,0.0001480959,0.000248509,0.00029158764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044654854,0.00028330745,0.0005349159,0.0005841258,0.0005997316,0.000981566,0.00020630244,0.00073521194,0.001613562],"category_scores_gemma":[0.0008618281,0.00011903652,0.00028978873,0.00039346307,0.00022051363,0.00038675868,0.0007396244,0.00082153425,0.0011001629],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002522451,0.0009808417,0.87676555,0.0002177422,0.00029220467,0.004378978,0.0019262827,0.003265205,0.05266841,0.0007448228,0.017789284,0.03844818],"study_design_scores_gemma":[0.000024820993,0.0003117182,0.98921824,0.00001594875,0.000046045225,0.00031490155,0.00039947653,0.0013912478,0.0033413584,0.000096657284,0.0048143947,0.000025162935],"about_ca_topic_score_codex":0.005006779,"about_ca_topic_score_gemma":0.0073095215,"teacher_disagreement_score":0.005006779,"about_ca_system_score_codex":0.0005121373,"about_ca_system_score_gemma":0.0002695614,"threshold_uncertainty_score":0.009955287},"labels":[],"label_agreement":null},{"id":"W3163863087","doi":"10.3847/1538-4357/ac478b","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: UV–Optical Accretion Disk Measurements with the Hubble Space Telescope","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Reverberation mapping; Quasar; Sky; Photometry (optics); Active galactic nucleus; Astronomy; Galaxy; Stars","score_opus":0.041201569538142746,"score_gpt":0.258986828277508,"score_spread":0.21778525873936527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3163863087","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99627614,0.00003324321,0.0007008163,0.000015823787,0.0000018625971,0.000010996384,0.0017763283,0.000071645685,0.001113151],"genre_scores_gemma":[0.9959853,0.00002431376,0.0012034148,0.00000984273,0.000005967191,0.000013257365,0.002418946,0.000011693226,0.00032723282],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998047,0.00004863201,0.000011484025,0.000039066894,0.00006707621,0.000029118899],"domain_scores_gemma":[0.99918133,0.00012251122,0.00029760707,0.00012307086,0.00013907517,0.00013624574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051536685,0.00026921157,0.00014712941,0.0011128309,0.0002344812,0.00030260737,0.00023750232,0.00013902054,0.0008985072],"category_scores_gemma":[0.0008588543,0.000117425036,0.00017970883,0.00054811157,0.00012419741,0.00016161452,0.00029023195,0.00016700003,0.00034669624],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002571079,0.000092225244,0.9764731,0.000023684748,0.00007734517,0.000107890024,0.00022947344,0.0024348907,0.0077712536,0.00012118365,0.0013389102,0.011073028],"study_design_scores_gemma":[0.0000082669285,0.000027359227,0.99540114,0.0000018853772,0.000009183519,0.000041208536,0.000026368632,0.0024803178,0.0015700746,0.00002062311,0.00041025982,0.0000032607418],"about_ca_topic_score_codex":0.009228032,"about_ca_topic_score_gemma":0.016339859,"teacher_disagreement_score":0.009228032,"about_ca_system_score_codex":0.00026137714,"about_ca_system_score_gemma":0.00015860159,"threshold_uncertainty_score":0.018348634},"labels":[],"label_agreement":null},{"id":"W3163906628","doi":"10.3847/1538-4357/ac133f","title":"The Atacama Cosmology Telescope: Microwave Intensity and Polarization Maps of the Galactic Center","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Lawrence Berkeley National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; National Institute of Standards and Technology; Science and Technology Facilities Council; University of Toronto; European Commission; Institut Périmètre de physique théorique; Flatiron Health; Industry Canada; National Science Foundation; Compute Canada; National Aeronautics and Space Administration; University of Pennsylvania; Princeton University; Gordon and Betty Moore Foundation; Government of Ontario; Ministry of Colleges and Universities; Government of Canada","keywords":"Physics; Galactic plane; Astrophysics; Cosmic microwave background; Galactic Center; Astronomy; Polarization (electrochemistry); Supernova remnant; Molecular cloud; Sky; Planck; Telescope; Intensity mapping; Pulsar wind nebula; Pulsar; Cosmology; Supernova; Galaxy; Redshift; Anisotropy; Stars; Optics","score_opus":0.007477141254253282,"score_gpt":0.2164459501624768,"score_spread":0.20896880890822353,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3163906628","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.948714,0.00090813945,0.003859771,0.00030334617,0.000028075343,0.00004088454,0.02072532,0.00077944575,0.024641119],"genre_scores_gemma":[0.97742677,0.00036286272,0.008679131,0.00006953091,0.00008033921,0.00002372215,0.011502378,0.00012065464,0.0017346612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999428,0.0000061897094,0.0000016645432,0.000014400483,0.000022267815,0.000012697406],"domain_scores_gemma":[0.99981505,0.00001384147,0.000044154327,0.000021582648,0.00005867818,0.000046840898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013782039,0.00015042748,0.00011817011,0.0027179683,0.0002512627,0.00047722796,0.00021376705,0.0001468799,0.002907238],"category_scores_gemma":[0.0001937914,0.00013739485,0.00017663681,0.0024885505,0.000113226815,0.00019469894,0.00031167155,0.00024705025,0.0005636074],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007303469,0.0002987576,0.6231046,0.00026987796,0.0004352084,0.00071329647,0.00084964454,0.008237292,0.14980036,0.003377304,0.038508423,0.17367485],"study_design_scores_gemma":[0.000012496691,0.000008698648,0.9909253,0.0000075704866,0.000013874284,0.00007669342,0.0000413403,0.0014423851,0.0013574373,0.00015571683,0.0059512267,0.0000070968413],"about_ca_topic_score_codex":0.01595928,"about_ca_topic_score_gemma":0.01743103,"teacher_disagreement_score":0.01595928,"about_ca_system_score_codex":0.00030549336,"about_ca_system_score_gemma":0.00018071353,"threshold_uncertainty_score":0.031732798},"labels":[],"label_agreement":null},{"id":"W3163951092","doi":"10.3847/1538-4357/ac4970","title":"Measuring Spin from Relative Photon-ring Sizes","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada; Ministero dello Sviluppo Economico; Gordon and Betty Moore Foundation; John Templeton Foundation; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada; Harvard University; Government of Canada; National Science Foundation","keywords":"Physics; Event horizon; Photon; Degeneracy (biology); Spin (aerodynamics); General relativity; Horizon; Astrophysics; Black hole (networking); Einstein ring; Degenerate energy levels; Event (particle physics); Quantum mechanics; Gravitational lens; Redshift; Classical mechanics; Astronomy; Galaxy","score_opus":0.03563082050721131,"score_gpt":0.3274551214597818,"score_spread":0.2918243009525705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3163951092","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9828857,0.00018067828,0.0082881,0.00003450845,0.000022029262,0.000007996333,0.0006314169,0.0000732658,0.007876339],"genre_scores_gemma":[0.9973972,0.000040194467,0.0020673417,0.000011180564,0.000012652515,0.0000049389773,0.00019370795,0.000008640048,0.00026421246],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997675,0.000052851356,0.000013590267,0.000073371666,0.00006161226,0.000031144617],"domain_scores_gemma":[0.9987264,0.00033759803,0.00038388153,0.00020241505,0.00021519863,0.00013449948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046973463,0.00015269552,0.00013835062,0.0009520783,0.0002203625,0.00067369564,0.00020489337,0.0001956734,0.0016668442],"category_scores_gemma":[0.002017604,0.00014251772,0.00009878985,0.00047484002,0.00031920298,0.00061253743,0.00056296476,0.000281976,0.0002199129],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086262904,0.0000817458,0.72287804,0.0001160222,0.00019177159,0.00014729337,0.00056441885,0.0037069384,0.16910955,0.0059270756,0.0015374881,0.09487702],"study_design_scores_gemma":[0.000024419305,0.00015673527,0.927893,0.000031132753,0.00008782767,0.00031002317,0.0003450314,0.012057502,0.052593265,0.0035469872,0.0029029052,0.00005113161],"about_ca_topic_score_codex":0.000592094,"about_ca_topic_score_gemma":0.0016606925,"teacher_disagreement_score":0.0016668442,"about_ca_system_score_codex":0.00022882434,"about_ca_system_score_gemma":0.00006414785,"threshold_uncertainty_score":0.0055761337},"labels":[],"label_agreement":null},{"id":"W3164418795","doi":"10.3847/1538-4357/ac0435","title":"Molecular Gas in a Gravitationally Lensed Galaxy Group at z = 2.9","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Agence Nationale de la Recherche","keywords":"Galaxy; Galaxy group; Peculiar galaxy; Galaxy cluster; Luminous infrared galaxy; Redshift; Population; Galaxy formation and evolution","score_opus":0.007847927874005806,"score_gpt":0.22953783230611666,"score_spread":0.22168990443211084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3164418795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951065,0.000021515563,0.000026866564,0.000010020257,7.1109406e-7,0.0000017085417,0.00015797254,0.0000056818917,0.00026485865],"genre_scores_gemma":[0.99953985,0.000011582545,0.00006844115,0.000006642922,0.0000028640964,0.0000012256103,0.00025553902,0.000001124548,0.00011274066],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999163,0.000009886338,0.000004441205,0.00002279504,0.000018077284,0.000028445147],"domain_scores_gemma":[0.9995253,0.00004399943,0.00020254104,0.000036216836,0.000058028538,0.00013395841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018249707,0.000170093,0.00020302644,0.0015027742,0.000316923,0.00037736513,0.00018595252,0.00014899824,0.0011282638],"category_scores_gemma":[0.000385218,0.00008834478,0.00013037001,0.0007371665,0.0002056071,0.00026801022,0.00041812114,0.00012425699,0.00019242207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000088010514,0.000027602402,0.9917265,0.0000042749994,0.000019975074,0.0000915553,0.00027437962,0.00007266316,0.0055725696,0.00006005958,0.00010914089,0.001953257],"study_design_scores_gemma":[0.0000010184767,0.000016992137,0.99950683,5.260032e-7,0.0000032767214,0.000033759625,0.00006386132,0.000098591096,0.00015848893,0.000012116398,0.00010374023,7.3025456e-7],"about_ca_topic_score_codex":0.012961482,"about_ca_topic_score_gemma":0.01222983,"teacher_disagreement_score":0.012961482,"about_ca_system_score_codex":0.00037677275,"about_ca_system_score_gemma":0.0000916705,"threshold_uncertainty_score":0.025772095},"labels":[],"label_agreement":null},{"id":"W3164550886","doi":"10.3847/1538-4357/ac35ec","title":"An Early-time Optical and Ultraviolet Excess in the Type-Ic SN 2020oi","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Ejecta; Supernova; Photometry (optics); Observatory; Astronomy; Luminosity; Stars; Galaxy","score_opus":0.008185086156779839,"score_gpt":0.2335024163202177,"score_spread":0.22531733016343786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3164550886","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989213,0.000038475897,0.000101558595,0.000004510748,9.3482566e-7,0.0000010557533,0.00011783734,0.000012295079,0.00080215634],"genre_scores_gemma":[0.99904567,0.00002562098,0.00014322353,0.000007035289,0.0000018612847,0.0000014553433,0.0004453478,0.0000027172491,0.0003270269],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999685,0.0000019705149,0.0000016799792,0.000009109579,0.000010170876,0.000008556229],"domain_scores_gemma":[0.9998722,0.000011188466,0.000048060978,0.000007214645,0.000018476643,0.000042816537],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009511586,0.00018506475,0.00009860171,0.00055853557,0.00014272211,0.00031809023,0.00011207261,0.00014056171,0.0011239359],"category_scores_gemma":[0.00018902622,0.000085586194,0.00009291563,0.0002896973,0.00009417121,0.00009622364,0.00018223954,0.00010835415,0.00021371651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003018298,0.00005480638,0.9055854,0.000024335777,0.000023082832,0.00048338197,0.00013554055,0.00020280734,0.08514176,0.00018976984,0.00026958462,0.007587584],"study_design_scores_gemma":[0.0000012333043,0.00004257461,0.9964515,0.0000019509887,0.0000061450587,0.0003252021,0.00004482936,0.00030022147,0.0024227884,0.000027155009,0.00037483493,0.0000015408382],"about_ca_topic_score_codex":0.0024282685,"about_ca_topic_score_gemma":0.005572072,"teacher_disagreement_score":0.0024282685,"about_ca_system_score_codex":0.00016915685,"about_ca_system_score_gemma":0.000055264125,"threshold_uncertainty_score":0.004828334},"labels":[],"label_agreement":null},{"id":"W3164715192","doi":"10.3847/1538-4357/ac32c9","title":"Sculpting the Sub-Saturn Occurrence Rate via Atmospheric Mass Loss","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Saturn; Stars; Astrophysics; Jovian; Accretion (finance); Astronomy; Planet","score_opus":0.006495225569932959,"score_gpt":0.19988507311415624,"score_spread":0.19338984754422328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3164715192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99628854,0.00009733606,0.0021962891,0.00004713926,0.00000255335,0.000002438697,0.00013327641,0.000043787823,0.0011886271],"genre_scores_gemma":[0.99959975,0.000022794453,0.00021174301,0.0000048108973,0.000002253984,9.333807e-7,0.000053916177,0.0000054172665,0.00009844166],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991584,0.00001180273,0.0000042614365,0.00003079183,0.000019951698,0.000017370063],"domain_scores_gemma":[0.9988832,0.00039023263,0.00043870867,0.000104947125,0.000088391025,0.00009457757],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003755161,0.00014312919,0.00013222115,0.0005572429,0.00018480448,0.00042535714,0.0002827969,0.00017388171,0.0011987557],"category_scores_gemma":[0.002203238,0.00010771923,0.00014585783,0.00028292928,0.00030333758,0.00040052016,0.0004046155,0.0002502891,0.00020153345],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015432805,0.000014695676,0.9553086,0.000028033272,0.00005168376,0.00013582048,0.00016203748,0.0046510156,0.02396038,0.0011239904,0.00020351748,0.014205847],"study_design_scores_gemma":[0.000004123992,0.000042752774,0.9482343,0.000007830642,0.00002282809,0.0002342222,0.00012230777,0.042755675,0.0067214193,0.0011713367,0.00067071785,0.00001236277],"about_ca_topic_score_codex":0.0035753134,"about_ca_topic_score_gemma":0.002469486,"teacher_disagreement_score":0.0035753134,"about_ca_system_score_codex":0.00039270124,"about_ca_system_score_gemma":0.00011893305,"threshold_uncertainty_score":0.007109046},"labels":[],"label_agreement":null},{"id":"W3165127413","doi":"10.3847/1538-4357/ac3820","title":"The Early Phases of Supernova 2020pni: Shock Ionization of the Nitrogen-enriched Circumstellar Material","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":65,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Division of Chemistry; Hong Kong Government; Gordon and Betty Moore Foundation; Nuclear Safety and Security Commission; National Research Foundation; Space Telescope Science Institute; Northwestern University; Villum Fonden; Canadian Institute for Advanced Research; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Supernova; Ionization; Astrophysics; Shock (circulatory); Shock wave; Nitrogen; Astronomy; Ion; Medicine","score_opus":0.008362138153037735,"score_gpt":0.2108553714621369,"score_spread":0.20249323330909916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3165127413","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9919411,0.00022653151,0.0008188486,0.00003522521,0.000017253285,0.000010730887,0.00071480527,0.00013208174,0.0061033806],"genre_scores_gemma":[0.99709344,0.000061054285,0.00039234734,0.000024268958,0.00000799005,0.000005824027,0.0014125695,0.00001798377,0.0009844933],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999658,0.0000022384916,0.0000013502568,0.000009017577,0.000010008418,0.000011606812],"domain_scores_gemma":[0.9999201,0.000007423545,0.000018435127,0.000007238438,0.000011527984,0.000035145105],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009341171,0.00029762316,0.00015883645,0.00029575854,0.00022160394,0.00031074588,0.00018825206,0.0002312715,0.0018103885],"category_scores_gemma":[0.00014732637,0.00012918918,0.00014796949,0.0002129239,0.00008608935,0.00013409651,0.0003507058,0.00027066414,0.00050505734],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020341112,0.00029911532,0.41275516,0.00023641117,0.00018710858,0.0046308455,0.00036868753,0.0045164097,0.5307504,0.0014331747,0.0059486553,0.036839932],"study_design_scores_gemma":[0.00002093085,0.00021423215,0.9620207,0.000016578046,0.0000239655,0.0013853022,0.000102429214,0.0063598747,0.02432061,0.0002441594,0.0052748495,0.000016263848],"about_ca_topic_score_codex":0.0022773165,"about_ca_topic_score_gemma":0.0029877876,"teacher_disagreement_score":0.0022773165,"about_ca_system_score_codex":0.0002561329,"about_ca_system_score_gemma":0.000076050026,"threshold_uncertainty_score":0.0060563684},"labels":[],"label_agreement":null},{"id":"W3166516562","doi":"10.3847/1538-4357/ac0f56","title":"A Spatially Resolved Survey of Distant Quasar Host Galaxies. I. Dynamics of Galactic Outflows","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Outflow; Quasar; Galaxy; Active galactic nucleus; Astronomy; Star formation; Redshift","score_opus":0.011203146900701467,"score_gpt":0.22377590091174307,"score_spread":0.21257275401104161,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3166516562","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990752,0.00014976939,0.00008076193,0.000017883887,0.0000012900674,0.0000025854317,0.00023612598,0.000007570977,0.0004287739],"genre_scores_gemma":[0.9991534,0.000094361945,0.00012735126,0.000014495582,0.000008912754,0.0000024799444,0.00040113155,0.0000023800267,0.0001955018],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998369,0.000020947486,0.000012703281,0.000056009107,0.000034107357,0.000039230792],"domain_scores_gemma":[0.9991725,0.000093458744,0.00037343946,0.000045244193,0.00007566946,0.00023970178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024169555,0.0002041391,0.00025388636,0.0014588326,0.00031636542,0.00049459597,0.00019562973,0.0002460714,0.0012729531],"category_scores_gemma":[0.00046643862,0.00017559534,0.00015344427,0.00084384554,0.00023033009,0.00043251686,0.00052618614,0.0002227555,0.0003355918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049358816,0.000041591808,0.98315954,0.000021116773,0.00003745657,0.00014201172,0.0003456621,0.00009105493,0.01087479,0.000109474735,0.00013739304,0.004990646],"study_design_scores_gemma":[0.0000019157508,0.000023599347,0.99928564,0.0000025281595,0.000005992025,0.000116942334,0.00007720148,0.00005598517,0.00016282461,0.00001257191,0.00025346197,0.000001394342],"about_ca_topic_score_codex":0.002976068,"about_ca_topic_score_gemma":0.0062926537,"teacher_disagreement_score":0.002976068,"about_ca_system_score_codex":0.00018709876,"about_ca_system_score_gemma":0.00009378908,"threshold_uncertainty_score":0.0059174895},"labels":[],"label_agreement":null},{"id":"W3166639361","doi":"10.3847/1538-4357/ac0623","title":"An Archival Search for Neutron-star Mergers in Gravitational Waves and Very-high-energy Gamma Rays","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Cherenkov radiation; Gravitational wave; Neutron star; Cherenkov Telescope Array; LIGO; Telescope; Binary number; Gamma-ray burst","score_opus":0.01180020825463619,"score_gpt":0.24676779982540242,"score_spread":0.23496759157076624,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3166639361","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961546,0.00006423173,0.0010377257,0.00003317104,0.000005689603,0.000022369131,0.0007469762,0.00005670652,0.0018785795],"genre_scores_gemma":[0.9920378,0.000054001925,0.0049889777,0.000018161061,0.000012627363,0.000012888048,0.0021527086,0.000016924532,0.00070587924],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981743,0.000019236018,0.000012837937,0.000046719524,0.000068263784,0.00003543553],"domain_scores_gemma":[0.99945253,0.000072746174,0.000155442,0.000086487475,0.000095746786,0.00013693867],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006426684,0.00012916283,0.00016289367,0.0021571836,0.0005112101,0.0007059503,0.00025930852,0.00019478379,0.00087992643],"category_scores_gemma":[0.00080208894,0.000110167595,0.0002331083,0.0013497607,0.00016650553,0.00030478294,0.00083847984,0.00022766074,0.00023086282],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000451434,0.000108177825,0.9331581,0.000045069348,0.00007224018,0.0004302584,0.0005305719,0.0012281265,0.025186725,0.0009502156,0.0016315114,0.036207575],"study_design_scores_gemma":[0.000022421846,0.00010946043,0.9807519,0.000022015403,0.000053194955,0.00030520489,0.000544847,0.008093625,0.0058841873,0.0003429818,0.0038557292,0.000014459219],"about_ca_topic_score_codex":0.0065452526,"about_ca_topic_score_gemma":0.022657793,"teacher_disagreement_score":0.0065452526,"about_ca_system_score_codex":0.000398823,"about_ca_system_score_gemma":0.00042330107,"threshold_uncertainty_score":0.013014317},"labels":[],"label_agreement":null},{"id":"W3166968866","doi":"10.3847/1538-4357/ac0ae3","title":"An Exquisitely Deep View of Quenching Galaxies through the Gravitational Lens: Stellar Population, Morphology, and Ionized Gas","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"European Research Council; Agence Nationale de la Recherche; Dunlap Institute for Astronomy and Astrophysics, University of Toronto","keywords":"Physics; Astrophysics; Quenching (fluorescence); Astronomy; Stellar population; Galaxy; Population; Morphology (biology); Gravitational lens; Gravitation; Star formation; Optics; Medicine","score_opus":0.012344926055955868,"score_gpt":0.24364901989859544,"score_spread":0.23130409384263959,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3166968866","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99863094,0.00017069583,0.00037975804,0.000018308614,4.8867827e-7,0.0000015494702,0.00007194623,0.000009627226,0.0007166592],"genre_scores_gemma":[0.9996251,0.00003462639,0.00012352045,0.00000731571,0.0000020617795,4.7058623e-7,0.000049492948,0.0000024568722,0.0001549264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999126,0.000010889878,0.000004129887,0.000022887381,0.000020937447,0.000028451661],"domain_scores_gemma":[0.99969256,0.000045429188,0.00012685232,0.00003168288,0.000032470336,0.00007110459],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019086922,0.00017659186,0.00019907736,0.0010274559,0.00024365692,0.00058249483,0.00016055255,0.00015993038,0.0010313144],"category_scores_gemma":[0.0003748796,0.00008764263,0.00014268687,0.0004898195,0.00033692888,0.0005321524,0.0004528992,0.00017419418,0.00019769275],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057593745,0.000017406115,0.95650434,0.000013037771,0.00002905847,0.00011126053,0.0006290049,0.00026825847,0.03149818,0.00039913165,0.00007496811,0.01039794],"study_design_scores_gemma":[4.714133e-7,0.00002010134,0.9984706,0.0000012533695,0.0000045589463,0.00007860228,0.0001585003,0.0002030272,0.00077580515,0.000093413575,0.00019226667,0.0000014276875],"about_ca_topic_score_codex":0.004529006,"about_ca_topic_score_gemma":0.0064559854,"teacher_disagreement_score":0.004529006,"about_ca_system_score_codex":0.00030895308,"about_ca_system_score_gemma":0.00007359211,"threshold_uncertainty_score":0.009005249},"labels":[],"label_agreement":null},{"id":"W3167041358","doi":"10.3847/1538-4357/ac289f","title":"Testing for Dark Matter in the Outskirts of Globular Clusters","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Globular cluster; Physics; Velocity dispersion; Astrophysics; Halo; Stars; Redshift; Galaxy; Cluster (spacecraft); Dark matter halo; Astronomy; Dark matter; RADIUS; Range (aeronautics); Dispersion (optics); Star cluster","score_opus":0.019977211808389683,"score_gpt":0.24830744509711314,"score_spread":0.22833023328872346,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3167041358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992742,0.000011705531,0.00022605527,0.000010915479,0.0000010509008,0.000001693452,0.00007517114,0.000008862956,0.00039024316],"genre_scores_gemma":[0.99971884,0.000002890297,0.000117569165,0.000003159396,6.869773e-7,4.3505068e-7,0.00008948012,0.0000028902693,0.00006400799],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99961394,0.00011494231,0.000017678018,0.00010691305,0.00007454117,0.000072054834],"domain_scores_gemma":[0.9962443,0.0015108174,0.0006699338,0.00032409062,0.00032492157,0.0009259235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008361477,0.0003486174,0.00033359413,0.0010901453,0.000708934,0.0009994593,0.0004965092,0.0002765684,0.0025508674],"category_scores_gemma":[0.0042618695,0.00019528049,0.000318234,0.00079343043,0.00061069155,0.0005707962,0.0007313636,0.00028667774,0.0002161068],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016422226,0.00001858237,0.9942194,0.0000072067924,0.00004086529,0.00008107356,0.00018579066,0.0012836169,0.002320995,0.00029183878,0.00007451515,0.0013117369],"study_design_scores_gemma":[0.000005628774,0.000049257615,0.99188215,0.0000054461134,0.000012689043,0.000043284286,0.0004578276,0.0055903904,0.0014209821,0.0003048407,0.00022168073,0.0000057829566],"about_ca_topic_score_codex":0.01460658,"about_ca_topic_score_gemma":0.017465014,"teacher_disagreement_score":0.01460658,"about_ca_system_score_codex":0.00055297255,"about_ca_system_score_gemma":0.0003165374,"threshold_uncertainty_score":0.029043138},"labels":[],"label_agreement":null},{"id":"W3167074237","doi":"10.3847/1538-4357/ac02c6","title":"Tracing PAH Size in Prominent Nearby Mid-Infrared Environments","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Universities Space Research Association","keywords":"Infrared; Physics; Astrophysics; Spectrograph; Ionization; Astronomy; Spectral line; Ion","score_opus":0.011297129388913049,"score_gpt":0.23452851878838124,"score_spread":0.22323138939946818,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3167074237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99895334,0.000040092655,0.00027916185,0.000005095139,6.472969e-7,0.0000022147276,0.00018693433,0.000027031516,0.0005054939],"genre_scores_gemma":[0.999206,0.000018126655,0.00037365162,0.0000054498337,0.0000014206304,0.000002906486,0.00027310292,0.0000042490324,0.000115065144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992716,0.0000057761686,0.0000017081912,0.000026419579,0.000019008561,0.000020051762],"domain_scores_gemma":[0.9997422,0.000034252986,0.0000846506,0.000021510534,0.000045014225,0.0000723794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000094035626,0.00015485933,0.00012726856,0.0009356822,0.00023957972,0.00032479886,0.00026038373,0.0002647197,0.00072682684],"category_scores_gemma":[0.00024596043,0.00012081127,0.00014265231,0.00039023353,0.00013555684,0.00024264498,0.0002962521,0.00018672575,0.00024640595],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018588807,0.000068387,0.868302,0.000020240817,0.00005004837,0.00019100792,0.00023725616,0.0011924233,0.119140126,0.00014699234,0.00019993629,0.0102657005],"study_design_scores_gemma":[0.0000017771096,0.000024533598,0.9940773,0.0000013805158,0.0000069592056,0.00007406436,0.00006173342,0.0012470555,0.0042122374,0.000025928886,0.00026341464,0.0000035121934],"about_ca_topic_score_codex":0.0038284042,"about_ca_topic_score_gemma":0.007276925,"teacher_disagreement_score":0.0038284042,"about_ca_system_score_codex":0.00025726753,"about_ca_system_score_gemma":0.00008254107,"threshold_uncertainty_score":0.0076122284},"labels":[],"label_agreement":null},{"id":"W3167153039","doi":"10.3847/1538-4357/ac05b9","title":"A Search for TeV Gamma-Ray Emission from Pulsar Tails by VERITAS","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Pulsar; Physics; Astrophysics; Luminosity; Gamma ray; Astronomy; Millisecond pulsar; Flux (metallurgy); Pulsar planet; Pulsar wind nebula; Binary pulsar; Stars; Nebula; Galaxy","score_opus":0.010988500685899337,"score_gpt":0.2453268152408442,"score_spread":0.23433831455494486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3167153039","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99741274,0.00015700722,0.0005551098,0.000027773216,0.0000038581857,0.0000037854204,0.00020151265,0.000027069169,0.0016111776],"genre_scores_gemma":[0.99856085,0.000058432128,0.0005148483,0.000037141046,0.000006478635,0.0000030853075,0.00048373843,0.000005670378,0.0003298619],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986017,0.000013841791,0.000007961166,0.000033945536,0.0000425028,0.000041433774],"domain_scores_gemma":[0.9989599,0.00032240697,0.00035814845,0.00009618865,0.00012549301,0.00013792337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003295232,0.00017475666,0.00016269778,0.0010814308,0.0003413066,0.00059696886,0.00029413687,0.00029456284,0.0019537786],"category_scores_gemma":[0.0007933763,0.00014950502,0.0001978636,0.0005157804,0.00027917046,0.00030292256,0.0006397655,0.00030642678,0.00030586726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041586507,0.000039615854,0.8490346,0.00004456833,0.000066376786,0.0011621399,0.00039163523,0.00033680542,0.13060212,0.0006918606,0.00032056606,0.016893933],"study_design_scores_gemma":[0.00001830064,0.00026530185,0.96809757,0.000035465488,0.00005259064,0.0025087951,0.00034011365,0.00147598,0.022979116,0.0007168165,0.0034911102,0.000018840357],"about_ca_topic_score_codex":0.00091577956,"about_ca_topic_score_gemma":0.0016004179,"teacher_disagreement_score":0.0019537786,"about_ca_system_score_codex":0.00015058693,"about_ca_system_score_gemma":0.00011384131,"threshold_uncertainty_score":0.0065360665},"labels":[],"label_agreement":null},{"id":"W3167316938","doi":"10.3847/1538-4357/ac23c6","title":"The Gravity Collective: A Search for the Electromagnetic Counterpart to the Neutron Star–Black Hole Merger GW190814","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Advanced Research","funders":"Fondo Nacional de Desarrollo Científico y Tecnológico; Science and Technology Facilities Council; Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España; Heising-Simons Foundation; National Aeronautics and Space Administration","keywords":"Physics; Neutron star; Astrophysics; Black hole (networking); Astronomy; Gravitational wave; Strong gravity; Gravitation","score_opus":0.012893799550713582,"score_gpt":0.3201689501540355,"score_spread":0.30727515060332194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3167316938","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873346,0.000030082363,0.0001706917,0.000029301415,0.0000018157356,0.0000035028204,0.00005994757,0.000009276352,0.00096198224],"genre_scores_gemma":[0.9993759,0.000019750958,0.00024749507,0.0000129238015,0.0000070327833,0.0000017316029,0.00018867583,0.0000028842371,0.00014372109],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999329,0.0000059937224,0.0000033423842,0.000017976634,0.000016638198,0.0000231151],"domain_scores_gemma":[0.999701,0.000022987286,0.00016765692,0.000022902273,0.00001807708,0.0000673423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016670793,0.00014055368,0.00014732622,0.0011814997,0.00048285528,0.00037396437,0.00018429365,0.00016898193,0.0014881131],"category_scores_gemma":[0.00028522927,0.00008824585,0.00015241811,0.00051205605,0.00025754242,0.00023699494,0.0006384316,0.00013919166,0.00017282911],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032146633,0.00007477271,0.93103206,0.000023689303,0.000058913858,0.0020925726,0.00044298978,0.00029193205,0.049576595,0.00056249433,0.00057296717,0.014949646],"study_design_scores_gemma":[0.0000077356235,0.00007337262,0.99604046,0.0000034000132,0.000018124127,0.0006098059,0.000310235,0.0005573294,0.0014247359,0.0001312498,0.0008187955,0.000004677079],"about_ca_topic_score_codex":0.0014770693,"about_ca_topic_score_gemma":0.0021505747,"teacher_disagreement_score":0.0014881131,"about_ca_system_score_codex":0.00021052125,"about_ca_system_score_gemma":0.00009762795,"threshold_uncertainty_score":0.0049782395},"labels":[],"label_agreement":null},{"id":"W3167755127","doi":"10.3847/1538-4357/ac5d4f","title":"A Study of 90 GHz Dust Emissivity on Molecular Cloud and Filament Scales","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Queen's University; University of Toronto","funders":"European Research Council","keywords":"Physics; Astrophysics; Photometry (optics); Black-body radiation; Protein filament; Molecular cloud; Emissivity; Spectral energy distribution; Planck; Astronomy; Star formation; Stars; Galaxy; Optics","score_opus":0.010948314032214489,"score_gpt":0.24567894619699382,"score_spread":0.23473063216477932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3167755127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999035,0.000030544772,0.0002665058,0.000017696024,8.005795e-7,0.0000011824826,0.0001392904,0.0000123564905,0.0004966673],"genre_scores_gemma":[0.9996536,0.000010206182,0.00012025794,0.0000034872864,0.0000027522483,7.902262e-7,0.00015192332,0.000003961673,0.00005306279],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999306,0.000008763163,0.000002521621,0.000022100074,0.000010290691,0.000025723575],"domain_scores_gemma":[0.99972326,0.00008756539,0.00007349069,0.00003036627,0.00003055492,0.000054727356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014425092,0.00011915509,0.00011587513,0.00052621245,0.00015622572,0.00032055276,0.0001588666,0.00014519456,0.00089757575],"category_scores_gemma":[0.00040184727,0.00008705855,0.00013217765,0.00043651243,0.00011736873,0.0002683664,0.00018467147,0.00017741986,0.00012941902],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001370715,0.00006080307,0.9369851,0.00001303283,0.00007271417,0.00015644237,0.00022861238,0.001191991,0.053100303,0.0003416447,0.00018343891,0.0075288136],"study_design_scores_gemma":[0.0000013497861,0.000009230475,0.9978961,0.0000011508878,0.00000619244,0.000023665063,0.000040427218,0.0011845873,0.00069210655,0.000030187935,0.00011353717,0.0000015998439],"about_ca_topic_score_codex":0.0032478478,"about_ca_topic_score_gemma":0.0030489813,"teacher_disagreement_score":0.0032478478,"about_ca_system_score_codex":0.00014305579,"about_ca_system_score_gemma":0.000036168065,"threshold_uncertainty_score":0.006457925},"labels":[],"label_agreement":null},{"id":"W3168104180","doi":"10.3847/1538-4357/ac0a75","title":"The Unusual Weak-line Quasar PG1407+265 and Its Foreground z ∼ 0.7 X-Ray Cluster","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science Mission Directorate","keywords":"Physics; Astrophysics; Quasar; Redshift; Cluster (spacecraft); Galaxy; Galaxy cluster; Photometry (optics); Astronomy; Eddington luminosity; Luminosity; Stars","score_opus":0.01012250355090456,"score_gpt":0.2280648913772206,"score_spread":0.21794238782631606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3168104180","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99852824,0.0000417719,0.00007220669,0.00002108127,0.0000029438154,0.0000020416276,0.000048273967,0.000009258256,0.0012741095],"genre_scores_gemma":[0.99949026,0.00002095185,0.00008348838,0.0000119614115,0.000008295562,8.573569e-7,0.00012199615,0.0000019956533,0.00026008498],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999527,0.0000015844488,0.0000012421156,0.000010795203,0.000014545593,0.000019160472],"domain_scores_gemma":[0.99987423,0.000006881743,0.000033210483,0.000008609672,0.000011750554,0.00006514811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000054543692,0.00014482855,0.00013175623,0.00039554367,0.0003750204,0.0003980053,0.0002607196,0.00012178982,0.0012753803],"category_scores_gemma":[0.0001318315,0.00009100385,0.0000764428,0.0002642182,0.00030363127,0.0001291771,0.00048769836,0.00018090905,0.00025744174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033590637,0.0001113903,0.88522303,0.000052280724,0.00005146714,0.011187807,0.0008087823,0.0004403394,0.07694921,0.0017469798,0.0017178021,0.02137507],"study_design_scores_gemma":[0.000006295702,0.00009022465,0.9925585,0.0000040172895,0.000013212319,0.0030179725,0.00027674696,0.00021376541,0.0012890309,0.00016644938,0.0023582296,0.0000055825362],"about_ca_topic_score_codex":0.0041222866,"about_ca_topic_score_gemma":0.0048074457,"teacher_disagreement_score":0.0041222866,"about_ca_system_score_codex":0.0002329299,"about_ca_system_score_gemma":0.00012895571,"threshold_uncertainty_score":0.008196592},"labels":[],"label_agreement":null},{"id":"W3168335801","doi":"10.3847/1538-4357/ac0913","title":"Supermassive Star Formation in Magnetized Atomic-cooling Gas Clouds: Enhanced Accretion, Intermittent Fragmentation, and Continuous Mergers","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Protostar; Supermassive black hole; Star formation; Angular momentum; Accretion (finance); Gravitational collapse; Magnetic field; Coalescence (physics)","score_opus":0.007067206689804589,"score_gpt":0.23343467523550845,"score_spread":0.22636746854570386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3168335801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965456,0.00018655011,0.0014649575,0.00014208317,0.000014103912,0.00001477181,0.000053213396,0.00002069899,0.0015580826],"genre_scores_gemma":[0.99946445,0.000058789043,0.00026622406,0.000018442566,0.000010494828,0.0000055209844,0.0000207866,0.0000039103484,0.0001513763],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999217,0.000020116873,0.0000028239538,0.000011731483,0.000011297949,0.00003228212],"domain_scores_gemma":[0.99958056,0.00013834589,0.000113970294,0.000020923568,0.000027463751,0.000118846394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024655822,0.00038014882,0.0005222283,0.00032352406,0.00067386904,0.0008153505,0.00079768366,0.0007381939,0.0012771531],"category_scores_gemma":[0.0008480448,0.00023962058,0.00057053997,0.0002694057,0.0008750657,0.000578838,0.0006502403,0.0004782095,0.00006853761],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004742034,0.0003108612,0.04068382,0.00009813928,0.00019140137,0.0012583757,0.00013750134,0.9295914,0.014227114,0.010306761,0.0005501559,0.0021701755],"study_design_scores_gemma":[0.00028312195,0.00013784136,0.014536004,0.000008331508,0.000043751013,0.0001071275,0.00007166135,0.98100543,0.0012300092,0.0022512684,0.00030967314,0.000015796079],"about_ca_topic_score_codex":0.0138007365,"about_ca_topic_score_gemma":0.0050441194,"teacher_disagreement_score":0.0138007365,"about_ca_system_score_codex":0.00085715344,"about_ca_system_score_gemma":0.0005209764,"threshold_uncertainty_score":0.027440846},"labels":[],"label_agreement":null},{"id":"W3169811235","doi":"10.3847/1538-4357/ac088b","title":"Inferring the Morphology of Stellar Distribution in TNG50: Twisted and Twisted-stretched Shapes","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Harvard University","keywords":"Physics; Astrophysics; Halo; Milky Way; Stars; Galaxy; Dark matter; Orientation (vector space); Angular momentum; Distribution (mathematics); Geometry; Classical mechanics","score_opus":0.008880490525546623,"score_gpt":0.2179503688125996,"score_spread":0.20906987828705298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3169811235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981219,0.00003063735,0.0008741546,0.000038689588,0.0000050399917,0.000004551643,0.00021878588,0.00007364076,0.00063265424],"genre_scores_gemma":[0.99816126,0.000013571371,0.0009943667,0.000018691893,0.0000028515994,0.000004831468,0.0006578521,0.00002501023,0.00012162497],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998605,0.000044599397,0.0000047481226,0.000031438216,0.000019099018,0.000039597715],"domain_scores_gemma":[0.99943167,0.00017546726,0.00005671219,0.00009723715,0.00008555197,0.00015331566],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061955134,0.00033262456,0.00035624192,0.00046257998,0.0003681293,0.00079386414,0.00092602434,0.0007756726,0.0013494914],"category_scores_gemma":[0.002338026,0.00022552707,0.0005791009,0.00038290865,0.00054234004,0.00033929758,0.0005782356,0.00032425218,0.00024725127],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023323053,0.00011026564,0.21305273,0.000041262436,0.00016424613,0.00040795177,0.00017475858,0.7738023,0.005579806,0.0011027585,0.00079441705,0.0045363116],"study_design_scores_gemma":[0.00006092161,0.00008243409,0.058005605,0.000013507191,0.000031894273,0.000087967055,0.00011482481,0.93923086,0.0013550859,0.00049892085,0.00050121424,0.00001675867],"about_ca_topic_score_codex":0.018281657,"about_ca_topic_score_gemma":0.011003172,"teacher_disagreement_score":0.018281657,"about_ca_system_score_codex":0.0005987552,"about_ca_system_score_gemma":0.0003535832,"threshold_uncertainty_score":0.03635049},"labels":[],"label_agreement":null},{"id":"W3169881194","doi":"10.3847/1538-4357/ac33ad","title":"No Evidence for Galactic Latitude Dependence of the Fast Radio Burst Sky Distribution","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Waterloo; University of Toronto; McGill University","funders":"Canada Foundation for Innovation","keywords":"Sky; Astrophysics; Physics; Latitude; Population; Range (aeronautics); Astronomy","score_opus":0.024978682213786973,"score_gpt":0.33929934887428514,"score_spread":0.3143206666604982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3169881194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9918532,0.0002038431,0.0033526463,0.00006114931,0.0000073436822,0.000010419734,0.0005415093,0.0000340303,0.0039359424],"genre_scores_gemma":[0.999329,0.000025961817,0.00019207149,0.000016022748,0.0000045607867,0.0000027485644,0.00024808772,0.000012601479,0.00016904146],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99778736,0.0005728583,0.0001586605,0.00064283743,0.00056683965,0.0002713441],"domain_scores_gemma":[0.98137164,0.007939342,0.0050348868,0.0028720933,0.0018807143,0.00090131443],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026579255,0.00016242528,0.00031806412,0.0010604494,0.00035920256,0.001036459,0.00040962585,0.0003167493,0.0047435765],"category_scores_gemma":[0.013717862,0.00018112583,0.00035826585,0.0008488051,0.0010399445,0.0004540202,0.00051041966,0.00027645082,0.0006806646],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025320332,0.000013712735,0.98576295,0.000022629447,0.00008904469,0.000069934846,0.00022714258,0.00030915497,0.0074582417,0.0005690896,0.00012984846,0.0050950893],"study_design_scores_gemma":[0.0000044408694,0.00003060062,0.99752825,0.000006370212,0.000023170438,0.00015227555,0.00013493362,0.00062698696,0.000882352,0.00024191909,0.0003610055,0.000007685526],"about_ca_topic_score_codex":0.0109656565,"about_ca_topic_score_gemma":0.012377587,"teacher_disagreement_score":0.0109656565,"about_ca_system_score_codex":0.0003487705,"about_ca_system_score_gemma":0.00033722227,"threshold_uncertainty_score":0.021803617},"labels":[],"label_agreement":null},{"id":"W3170304536","doi":"10.3847/1538-4357/ac347e","title":"Simulating Globular Clusters in Dark Matter Subhalos","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Halo; Velocity dispersion; Globular cluster; Dark matter halo; RADIUS; Dark matter; Virial theorem; Virial mass; Milky Way; Redshift; Astronomy; Galaxy","score_opus":0.013005115209877505,"score_gpt":0.24485975410623997,"score_spread":0.23185463889636246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3170304536","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944066,0.00004514542,0.0018749494,0.00012447483,0.00001920079,0.000025833546,0.0003804388,0.00020521392,0.0029182096],"genre_scores_gemma":[0.99339104,0.00005005058,0.004167431,0.00006744021,0.000009145563,0.000035131463,0.00079135475,0.00006938716,0.001419007],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998727,0.000037067577,0.000003979075,0.000024241353,0.000019679683,0.00004244488],"domain_scores_gemma":[0.9991804,0.00034514166,0.00006436578,0.00006935377,0.000095701726,0.00024511394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043597806,0.00047468502,0.0005004527,0.0004837054,0.0006266396,0.00081589684,0.0016038525,0.0009642003,0.0031463532],"category_scores_gemma":[0.0018195127,0.0003280112,0.00059072365,0.00065104326,0.00078623625,0.00064558035,0.001042822,0.00075957214,0.00024296329],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028669677,0.00018695895,0.016734395,0.000028989414,0.00008086253,0.00018300289,0.00018502539,0.9748268,0.0011773667,0.0038288806,0.00074737245,0.0017337046],"study_design_scores_gemma":[0.00014772336,0.000053008913,0.0030397144,0.000005227921,0.000016663664,0.000014082915,0.000081833605,0.99410975,0.00056322344,0.0010797592,0.000879542,0.000009577555],"about_ca_topic_score_codex":0.05452671,"about_ca_topic_score_gemma":0.030353915,"teacher_disagreement_score":0.05452671,"about_ca_system_score_codex":0.0017814315,"about_ca_system_score_gemma":0.0010354542,"threshold_uncertainty_score":0.10841864},"labels":[],"label_agreement":null},{"id":"W3170384143","doi":"10.3847/1538-4357/ac2fa8","title":"Rare Event Sampling Improves Mercury Instability Statistics","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Scientific Research and Discoveries","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Advanced Scientific Computing Research; Nuclear Safety and Security Commission; York University; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Rare events; Importance sampling; Instability; Event (particle physics); Monte Carlo method; Mercury (programming language); Quantile; Sampling (signal processing); Statistical physics; Statistics; Computer science; Meteorology; Econometrics; Mathematics; Physics; Mechanics","score_opus":0.022553742462825713,"score_gpt":0.30468404698495793,"score_spread":0.2821303045221322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3170384143","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.21480812,0.00072984304,0.77855504,0.0005051051,0.00009925481,0.000072330986,0.00034068787,0.002536852,0.0023527693],"genre_scores_gemma":[0.9012584,0.00016539377,0.09679335,0.00015507257,0.000070417685,0.000041383988,0.000489297,0.00020293903,0.0008237558],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989054,0.00055357494,0.000040925494,0.00017525817,0.0002357331,0.00008896775],"domain_scores_gemma":[0.96799445,0.025591865,0.0012167861,0.0028488606,0.0018469685,0.00050104666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003994397,0.00041108872,0.0008067602,0.0012472454,0.0005752224,0.00085834385,0.0010918556,0.0005661708,0.0018624504],"category_scores_gemma":[0.031430908,0.00034467917,0.00042855964,0.0006976999,0.000818571,0.0011552866,0.001123565,0.0011004417,0.00032474438],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036158148,0.00010918195,0.032311358,0.000117134914,0.00013661444,0.00018780598,0.00013160528,0.86962575,0.0043920986,0.034497492,0.0025504942,0.055578973],"study_design_scores_gemma":[0.0000069513894,0.000010888033,0.0005940539,0.0000039458146,0.000004007368,0.000017526512,0.0000055443293,0.9946839,0.00075542665,0.0036994768,0.00021336356,0.0000049342398],"about_ca_topic_score_codex":0.012760641,"about_ca_topic_score_gemma":0.009249891,"teacher_disagreement_score":0.012760641,"about_ca_system_score_codex":0.0008362696,"about_ca_system_score_gemma":0.00125261,"threshold_uncertainty_score":0.025372744},"labels":[],"label_agreement":null},{"id":"W3170884957","doi":"10.3847/1538-4357/ac06c7","title":"Ionized Gas Outflows in Low-excitation Radio Galaxies Are Radiation Driven","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; University of Manitoba","funders":"","keywords":"Sky; Active galactic nucleus; Outflow; Quasar; Accretion (finance); Galaxy; Ionization; Radio galaxy; Radiation pressure","score_opus":0.006292493790762097,"score_gpt":0.2078882388460528,"score_spread":0.20159574505529068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3170884957","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999275,0.000050867504,0.00017439168,0.0000062368786,9.742209e-7,0.0000018003799,0.00005256551,0.000013321352,0.00042489637],"genre_scores_gemma":[0.9996117,0.00003131019,0.000112180736,0.000009134255,0.0000033796975,0.0000011819111,0.00013980572,0.000002239789,0.00008916694],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988425,0.000011319429,0.000008340861,0.00003625694,0.000017862698,0.000041887022],"domain_scores_gemma":[0.9993426,0.000069247646,0.00038269346,0.000039817718,0.000044344535,0.00012130356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020759925,0.00019995417,0.00016813508,0.0010722158,0.0001992289,0.0008107136,0.00021090376,0.00017300619,0.001307411],"category_scores_gemma":[0.00045355523,0.00011744352,0.00015221158,0.00043375944,0.00040586098,0.00026033283,0.00041688932,0.0001292089,0.0002785996],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003817899,0.000019648829,0.9905996,0.000010871345,0.000013706828,0.0001729949,0.00011313,0.00011319863,0.006702386,0.0001161465,0.00008571312,0.0020143574],"study_design_scores_gemma":[0.0000018715696,0.00001844988,0.99862766,0.0000031189716,0.00000774392,0.00019847222,0.000105747815,0.00020946478,0.0005975801,0.000051283452,0.0001767752,0.0000017678192],"about_ca_topic_score_codex":0.0010662631,"about_ca_topic_score_gemma":0.0012028712,"teacher_disagreement_score":0.001307411,"about_ca_system_score_codex":0.00017430402,"about_ca_system_score_gemma":0.000056087807,"threshold_uncertainty_score":0.0043736696},"labels":[],"label_agreement":null},{"id":"W3171615221","doi":"10.3847/1538-4357/abf926","title":"VERITAS Observations of the Galactic Center Region at Multi-TeV Gamma-Ray Energies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Division of Physics; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Galactic Center; Gamma ray; Astrophysics; Astronomy; Gamma-ray astronomy; Center (category theory); Galaxy","score_opus":0.02336157954562356,"score_gpt":0.2267255550996116,"score_spread":0.20336397555398802,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3171615221","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99655616,0.00014325423,0.00026158028,0.000015604672,0.0000047895023,0.0000050420726,0.0009806788,0.00007162893,0.0019612582],"genre_scores_gemma":[0.9969969,0.00005387814,0.0006655439,0.000015306494,0.000008923373,0.0000037287869,0.001754173,0.000019721312,0.00048194855],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982613,0.000010871886,0.0000059994413,0.000053407206,0.000065368265,0.00003831495],"domain_scores_gemma":[0.9996493,0.00003818434,0.00012724471,0.000047356814,0.00006210876,0.00007575634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002160217,0.00022398394,0.00020884047,0.0014807576,0.00028466855,0.00053885573,0.00031579018,0.00023272146,0.00093199336],"category_scores_gemma":[0.00027424542,0.00016849091,0.0002751941,0.00080578146,0.0001281644,0.00021728779,0.00046447752,0.00025287678,0.0002176741],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040853626,0.000058135276,0.8584549,0.000042364187,0.0002116376,0.0005234336,0.0003285395,0.0010812696,0.12483441,0.00026354153,0.0008863472,0.012906943],"study_design_scores_gemma":[0.0000064660994,0.00003330906,0.9954869,0.0000053302583,0.000026930855,0.00012932236,0.000060722967,0.00053984154,0.0025198464,0.000024383773,0.0011619205,0.0000049745954],"about_ca_topic_score_codex":0.01173597,"about_ca_topic_score_gemma":0.030790359,"teacher_disagreement_score":0.01173597,"about_ca_system_score_codex":0.00041539953,"about_ca_system_score_gemma":0.0001642611,"threshold_uncertainty_score":0.023335338},"labels":[],"label_agreement":null},{"id":"W3171807859","doi":"10.3847/1538-4357/ac0ae2","title":"The Diversity of Environments around Luminous Quasars at Redshift z ∼ 6","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Physics; Astrophysics; Galaxy; Halo; Redshift; Dark matter; Sigma; Astronomy; Luminosity","score_opus":0.008554461305768942,"score_gpt":0.1962290563844408,"score_spread":0.18767459507867185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3171807859","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989944,0.000026581309,0.00044669965,0.000049977418,0.0000011865046,0.0000017768433,0.00012607098,0.000019085548,0.00033416811],"genre_scores_gemma":[0.9995441,0.000017365031,0.0001495734,0.000009132402,0.0000017764092,9.47823e-7,0.00017533526,0.000003904463,0.00009779447],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998714,0.00002342408,0.0000055348746,0.000046655212,0.000020806132,0.00003219911],"domain_scores_gemma":[0.99924964,0.00014714949,0.00024937192,0.000083447114,0.00006438295,0.00020606768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003725512,0.00015327333,0.00022407215,0.00067806605,0.00033819766,0.0010510815,0.00056241394,0.00029669335,0.0019602252],"category_scores_gemma":[0.0015278814,0.00019661673,0.0003042073,0.00036222851,0.00061721384,0.00048027321,0.0007411484,0.00032992303,0.0001635121],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018626112,0.000067910776,0.9111757,0.000024093926,0.00010667208,0.00018772218,0.0005417808,0.06556586,0.010717465,0.0054874383,0.0007450552,0.0051940223],"study_design_scores_gemma":[0.000043087828,0.00013321261,0.9039788,0.000017855207,0.00005610924,0.00027380232,0.000540835,0.08785628,0.0015576279,0.004513587,0.0009987451,0.000030003022],"about_ca_topic_score_codex":0.007252553,"about_ca_topic_score_gemma":0.010140348,"teacher_disagreement_score":0.007252553,"about_ca_system_score_codex":0.00038169432,"about_ca_system_score_gemma":0.00013376294,"threshold_uncertainty_score":0.014420688},"labels":[],"label_agreement":null},{"id":"W3172428071","doi":"10.3847/1538-4357/abfa9a","title":"The Search for Binary Supermassive Black Holes among Quasars with Offset Broad Lines Using the Very Long Baseline Array","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Supermassive black hole; Physics; Astrophysics; Quasar; Very Long Baseline Array; Active galactic nucleus; Binary number; Sky; Astronomy; Galaxy","score_opus":0.014443367250040225,"score_gpt":0.24548530027460083,"score_spread":0.2310419330245606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3172428071","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953852,0.00024271561,0.0027218594,0.00006840522,0.0000054017205,0.000009647644,0.00021383046,0.00006639426,0.0012863518],"genre_scores_gemma":[0.9975485,0.000030547908,0.001954534,0.000029645316,0.000010911594,0.000003205944,0.00027578755,0.0000040986743,0.00014270046],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996288,0.00007826281,0.000015007625,0.00010725063,0.00009295135,0.00007775951],"domain_scores_gemma":[0.99843174,0.00025325603,0.00063100585,0.00011231771,0.0001624201,0.00040909482],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072446564,0.00015599321,0.00018892223,0.0014385318,0.00037597297,0.00082544825,0.00032694312,0.00024502652,0.00173033],"category_scores_gemma":[0.0008794646,0.00016172828,0.00018228976,0.0007051458,0.0002064156,0.00051322,0.00060455553,0.00023544338,0.0002875611],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000117212825,0.000050024923,0.9570658,0.00001967585,0.00009097179,0.00020210845,0.00015509897,0.00027083917,0.027404822,0.00036568538,0.00035023567,0.013907526],"study_design_scores_gemma":[0.000009276302,0.00011358819,0.9943811,0.0000070393608,0.000035941248,0.000335931,0.00022812239,0.0019000287,0.0018963555,0.00022872604,0.0008565456,0.0000074295326],"about_ca_topic_score_codex":0.0009874268,"about_ca_topic_score_gemma":0.002800714,"teacher_disagreement_score":0.00173033,"about_ca_system_score_codex":0.00016742382,"about_ca_system_score_gemma":0.00012304913,"threshold_uncertainty_score":0.005788505},"labels":[],"label_agreement":null},{"id":"W3172758318","doi":"","title":"A Coordinated X-Ray and Optical Campaign of the Nearby Massive Binary Sigma Orionis Aa","year":2015,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec","funders":"","keywords":"Physics; Astrophysics; Flux (metallurgy); Radiative transfer; Spectral line; Emission spectrum; Binary number; Line (geometry); Orbital period; Binary star; Amplitude; Light curve; X-ray binary; Be star; Variable star; Phase (matter); Astronomy; Stars; Neutron star; Optics","score_opus":0.015577241007949714,"score_gpt":0.22908196106494952,"score_spread":0.2135047200569998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3172758318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9921212,0.00012462001,0.0010195876,0.000035628484,0.000012290678,0.000045200584,0.0051421546,0.00016749748,0.0013318604],"genre_scores_gemma":[0.9710189,0.0001878884,0.004963375,0.000042674023,0.00006485835,0.000060808623,0.0226028,0.000088468936,0.00097027863],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972695,0.000029469125,0.000014976557,0.000115159615,0.000065752785,0.000047609654],"domain_scores_gemma":[0.99929035,0.000055935052,0.00019888785,0.0001359916,0.00010247412,0.00021634685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037837142,0.00042952958,0.0003445809,0.0016751487,0.00061983836,0.0005427056,0.00031520062,0.00026362334,0.0008293442],"category_scores_gemma":[0.00047004034,0.00023395084,0.00034197595,0.001492445,0.00025003843,0.00032111278,0.0007196523,0.00027176464,0.0003933856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001421972,0.0012812603,0.7844931,0.0003253587,0.00048082974,0.0021530436,0.002000565,0.008088626,0.12490293,0.0008858897,0.005253252,0.06871327],"study_design_scores_gemma":[0.000028972909,0.00016080143,0.99118793,0.0000062610825,0.00004634527,0.00025121367,0.00012711248,0.0019164779,0.0018889703,0.00010653767,0.0042678923,0.000011463506],"about_ca_topic_score_codex":0.011237978,"about_ca_topic_score_gemma":0.020037599,"teacher_disagreement_score":0.011237978,"about_ca_system_score_codex":0.000365953,"about_ca_system_score_gemma":0.0005412277,"threshold_uncertainty_score":0.022345126},"labels":[],"label_agreement":null},{"id":"W3172792549","doi":"10.3847/1538-4357/ac1dab","title":"CHIME/FRB Catalog 1 Results: Statistical Cross-correlations with Large-scale Structure","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of British Columbia; Canadian Institute for Theoretical Astrophysics; McGill University; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Fonds de recherche du Québec – Nature et technologies; National Defense Science and Engineering Graduate; Office of Science; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; McGill Space Institute; Killam Trusts; National Research Council Canada; University of Toronto; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Research Chairs; Industry Canada; Canada Foundation for Innovation; National Science Foundation; Compute Canada; U.S. Department of Defense; U.S. Department of Energy; McGill University; High Energy Physics; Smithsonian Astrophysical Observatory; Western Canada Research Grid; Canadian Institute for Advanced Research; Government of Canada","keywords":"Redshift; Halo; Galaxy; Dark matter; Population; Galaxy formation and evolution; Dark matter halo","score_opus":0.004714115110125898,"score_gpt":0.22513248155131976,"score_spread":0.22041836644119386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3172792549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92839295,0.000578457,0.0051173,0.00022858559,0.000026806441,0.000072890536,0.05699456,0.0013161347,0.0072723683],"genre_scores_gemma":[0.9426883,0.00008162939,0.0023360043,0.00008011622,0.000044275526,0.0000626891,0.0528983,0.00029782404,0.0015109659],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9972601,0.00053714064,0.00018475244,0.0007372626,0.0009018101,0.00037887812],"domain_scores_gemma":[0.97777903,0.010489091,0.003791233,0.003907907,0.0029180327,0.0011146278],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00419579,0.0005657066,0.0006566431,0.0056503685,0.0005593464,0.0020326753,0.00052666856,0.00044942295,0.008525866],"category_scores_gemma":[0.018171376,0.00022036144,0.0007700653,0.004829206,0.00041907324,0.0007604669,0.0013766341,0.00045128333,0.0022928198],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016411161,0.000036449823,0.98162216,0.000053218806,0.00040478492,0.00008430333,0.00006729181,0.0020104854,0.0012757108,0.00035545806,0.0066853305,0.0072407573],"study_design_scores_gemma":[0.000014049432,0.000019388013,0.9933582,0.000008047738,0.000047619993,0.000076271914,0.00005696101,0.003448474,0.00080146856,0.00014327579,0.0020107254,0.000015556836],"about_ca_topic_score_codex":0.0142798005,"about_ca_topic_score_gemma":0.011358089,"teacher_disagreement_score":0.0142798005,"about_ca_system_score_codex":0.0005871237,"about_ca_system_score_gemma":0.00047331283,"threshold_uncertainty_score":0.028521895},"labels":[],"label_agreement":null},{"id":"W3172848651","doi":"10.3847/1538-4357/ac0723","title":"No Impact of Core-scale Magnetic Field, Turbulence, or Velocity Gradient on Sizes of Protostellar Disks in Orion A","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Ministry of Science and Technology, Taiwan","keywords":"Physics; Astrophysics; Magnetic field; Turbulence; Magnetohydrodynamics; Velocity gradient; Millimeter; Submillimeter Array; Angular velocity; Computational physics; Star formation; Stars; Mechanics; Classical mechanics","score_opus":0.013804383270136701,"score_gpt":0.26837203081350686,"score_spread":0.25456764754337013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3172848651","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99978846,0.000021915943,0.000030231602,0.0000050891376,6.605846e-7,5.5553534e-7,0.00005148825,0.0000027135986,0.00009884165],"genre_scores_gemma":[0.99989223,0.0000044780563,0.000017685687,0.0000023139446,0.0000010024527,7.530318e-7,0.00004933866,0.000001557137,0.000030760108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998349,0.00003479529,0.00001300691,0.000070594346,0.000020448111,0.000026231068],"domain_scores_gemma":[0.998415,0.00055888935,0.00036435822,0.00017898552,0.000120072975,0.0003626668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022007525,0.00018899792,0.00019632261,0.0004582509,0.00025337056,0.0005721012,0.00025986612,0.00021517681,0.0010273948],"category_scores_gemma":[0.0016194121,0.000099015815,0.00015317398,0.00016507378,0.0003426802,0.00034086063,0.00040054746,0.00014529191,0.00012868829],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042832587,0.00005959714,0.96582985,0.000018196166,0.00006410319,0.0001484987,0.00014125348,0.0010753908,0.029571077,0.00010762202,0.00005984951,0.0024962141],"study_design_scores_gemma":[0.000004195385,0.000043133245,0.99790764,0.0000015007461,0.000008761997,0.000042560736,0.00011056621,0.0007737803,0.00096826965,0.000050340226,0.000086581866,0.0000027569456],"about_ca_topic_score_codex":0.0020227674,"about_ca_topic_score_gemma":0.0016832206,"teacher_disagreement_score":0.0020227674,"about_ca_system_score_codex":0.0002390011,"about_ca_system_score_gemma":0.00010536665,"threshold_uncertainty_score":0.0040219426},"labels":[],"label_agreement":null},{"id":"W3173145356","doi":"10.3847/1538-4357/ac0c81","title":"Back to Quiescence: Postoutburst Evolution of the Pulsar J1119–6127 and Its Wind Nebula","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Canadian Space Agency; National Science Foundation","keywords":"Nebula; Pulsar; Astronomy; Physics; Biology; Stars","score_opus":0.010216872433989404,"score_gpt":0.22669145359796802,"score_spread":0.2164745811639786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3173145356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986847,0.00008117598,0.000113931594,0.00003177124,0.000006431284,0.000004042123,0.00023271365,0.000015215439,0.0008300102],"genre_scores_gemma":[0.99794644,0.00006095363,0.00014541317,0.000023171619,0.000009084285,0.0000044174535,0.0010518938,0.00001415764,0.00074459997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999206,0.0000075479566,0.0000032429846,0.000022447917,0.000020544396,0.000025619416],"domain_scores_gemma":[0.9996352,0.00006545121,0.000084319756,0.000038451548,0.00007401699,0.000102518585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014323035,0.00020984269,0.00033285108,0.0005086753,0.000436758,0.0006381046,0.0002522293,0.00025025188,0.001170413],"category_scores_gemma":[0.00065038126,0.00015401228,0.00019638272,0.00044779366,0.0002623456,0.00029137923,0.0004341193,0.00047138147,0.0004310261],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00057518214,0.0003152938,0.9072897,0.000070064045,0.00014038605,0.0032525142,0.0006602737,0.0016401752,0.06343229,0.00050635875,0.0014991214,0.020618629],"study_design_scores_gemma":[0.000008158243,0.000057929916,0.9951002,0.0000045218103,0.000017214745,0.00033417472,0.00018377723,0.00096054334,0.0015674855,0.000070791175,0.001685467,0.000009779432],"about_ca_topic_score_codex":0.010759137,"about_ca_topic_score_gemma":0.020565545,"teacher_disagreement_score":0.010759137,"about_ca_system_score_codex":0.00050755794,"about_ca_system_score_gemma":0.00023419209,"threshold_uncertainty_score":0.02139306},"labels":[],"label_agreement":null},{"id":"W3173237844","doi":"10.3847/1538-4357/ac0e9d","title":"Resolving the Formation of Cold H i Filaments in the High-velocity Cloud Complex C","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Halo; Astrophysics; Star formation; Galaxy; Milky Way; Turbulence; Galactic halo; Meteorology","score_opus":0.032781607762666795,"score_gpt":0.2922864928586882,"score_spread":0.2595048850960214,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3173237844","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992773,0.000029459325,0.00039699304,0.00000739664,0.0000010087091,0.000002647216,0.0000763743,0.0000096643025,0.00019921252],"genre_scores_gemma":[0.9994821,0.000012945578,0.00035805488,0.000002537469,0.0000020418713,0.0000010143126,0.0000988223,0.000002196206,0.000040263814],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994147,0.0000047322,0.0000024421734,0.000015964277,0.000011436247,0.000024037345],"domain_scores_gemma":[0.9997427,0.000047778696,0.00008137947,0.000016433722,0.000038209288,0.000073398194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001293715,0.00015171242,0.00014056641,0.0011149427,0.00037598444,0.0005994104,0.00020235911,0.00026117015,0.0005687493],"category_scores_gemma":[0.0003781044,0.00010413048,0.00015564865,0.0005661451,0.00024208923,0.00029557504,0.0002985576,0.00015017955,0.00007901611],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026511535,0.0001287443,0.859502,0.000056326666,0.00008638111,0.0004518518,0.0004470552,0.013593876,0.108747624,0.0009882674,0.00050578057,0.015226996],"study_design_scores_gemma":[0.0000051614015,0.00002731694,0.9609588,0.0000053993203,0.00001013382,0.00005939606,0.00022158767,0.034542512,0.0037494944,0.00015102436,0.00026092958,0.000008275465],"about_ca_topic_score_codex":0.01078704,"about_ca_topic_score_gemma":0.010815791,"teacher_disagreement_score":0.01078704,"about_ca_system_score_codex":0.00040141118,"about_ca_system_score_gemma":0.0002127143,"threshold_uncertainty_score":0.021448493},"labels":[],"label_agreement":null},{"id":"W3174650889","doi":"10.3847/1538-4357/ac0c7e","title":"Long Term Evolution of Surface Features on the Red Supergiant AZ Cyg","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"European Space Agency; Office of the Vice President for Research and Economic Development, University at Buffalo; California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Red supergiant; RADIUS; Supergiant; Spectral line; Astronomy; Stellar evolution; Infrared telescope; Stars; Angular diameter; Telescope; Line (geometry); Geometry","score_opus":0.009431057236474971,"score_gpt":0.21810597079864683,"score_spread":0.20867491356217185,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3174650889","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997832,0.00012945232,0.00022626009,0.00004560245,0.0000034638247,0.000002672448,0.0005259473,0.000037458147,0.0011971636],"genre_scores_gemma":[0.9989556,0.00003124148,0.00011004985,0.000010403598,0.000006741357,0.0000019299068,0.000692996,0.000010142217,0.00018083675],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998871,0.000009099746,0.000004227378,0.000038043756,0.00003419261,0.000027343025],"domain_scores_gemma":[0.99947673,0.00008760627,0.00018149066,0.00005936098,0.00008863438,0.00010623698],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031297575,0.00023560147,0.00021504516,0.0008339678,0.00032162046,0.00053137797,0.0002225135,0.0003144964,0.00091549946],"category_scores_gemma":[0.0008402906,0.0001490015,0.00026600496,0.00061863085,0.00036750265,0.00045486368,0.0005348631,0.0003379034,0.00025443497],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021092583,0.000051599665,0.9496437,0.000030071911,0.00016210307,0.00025758828,0.0002634894,0.0038000324,0.033678688,0.0003907541,0.0009891836,0.010521816],"study_design_scores_gemma":[0.0000012686061,0.000011737965,0.99797755,0.0000017448792,0.00000798201,0.000020231739,0.000020255195,0.0010125411,0.00062571594,0.000027455582,0.0002901593,0.0000033733877],"about_ca_topic_score_codex":0.0075049885,"about_ca_topic_score_gemma":0.008257997,"teacher_disagreement_score":0.0075049885,"about_ca_system_score_codex":0.0007383195,"about_ca_system_score_gemma":0.00011886706,"threshold_uncertainty_score":0.014922619},"labels":[],"label_agreement":null},{"id":"W3174657702","doi":"10.3847/1538-4357/ac0bb6","title":"Radial Gradients in Dust-to-gas Ratio Lead to Preferred Region for Giant Planet Formation","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Space Telescope Science Institute","keywords":"Physics; Astrophysics; Opacity; Protoplanetary disk; Planet; Accretion (finance); Interstellar medium; Gas giant; Giant planet; Planetary system; Exoplanet; Galaxy","score_opus":0.028682799159239887,"score_gpt":0.26106903405853416,"score_spread":0.23238623489929428,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3174657702","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99906737,0.00003938838,0.00043014938,0.000012160165,0.0000010590976,0.0000015610826,0.000059985803,0.00002591812,0.00036238687],"genre_scores_gemma":[0.9997651,0.000008524145,0.00010792813,0.000002962081,5.9010597e-7,9.123534e-7,0.000030671872,0.00000420836,0.00007913069],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999956,0.0000053732056,0.000002560492,0.00001811224,0.0000050530584,0.000012974476],"domain_scores_gemma":[0.9996835,0.000099935816,0.000094779265,0.000025913976,0.000029360406,0.000066616885],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007860299,0.000104513485,0.0001385579,0.00025242488,0.00014672172,0.0003333064,0.0001584533,0.00019084793,0.0012420216],"category_scores_gemma":[0.00077009504,0.00015280594,0.00013055214,0.00010300877,0.00015377192,0.00011254393,0.00020516002,0.0001879739,0.00020950822],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009605177,0.00005864003,0.49828848,0.00004962747,0.00008416876,0.00092161866,0.00013520518,0.010899652,0.47970983,0.00074667204,0.0003373098,0.0078081572],"study_design_scores_gemma":[0.000015157075,0.00010794309,0.9593337,0.0000057400657,0.000027616685,0.0005248887,0.00015772542,0.01566532,0.023353651,0.0003932131,0.00040402007,0.000010938753],"about_ca_topic_score_codex":0.0020944702,"about_ca_topic_score_gemma":0.001939542,"teacher_disagreement_score":0.0020944702,"about_ca_system_score_codex":0.00023053003,"about_ca_system_score_gemma":0.00011164904,"threshold_uncertainty_score":0.004164517},"labels":[],"label_agreement":null},{"id":"W3175094828","doi":"10.3847/1538-4357/acd2d5","title":"Physics and Chemistry of Radiation Driven Cloud Evolution. [C ii] Kinematics of IC 59, and IC 63","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Aeronautics and Space Administration; Universität Stuttgart; Science and Technology Facilities Council; University of Hertfordshire; Universities Space Research Association; National Science Foundation","keywords":"Physics; Nebula; Astrophysics; Magnetic field; Orion Nebula; Kinetic energy; Star formation; Radiation; Galaxy; Stars; Optics","score_opus":0.007774722413214304,"score_gpt":0.2259764478198458,"score_spread":0.2182017254066315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3175094828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99526536,0.00031814424,0.00061567914,0.000070268485,0.0000068641734,0.000020437987,0.00022546813,0.00003242166,0.003445293],"genre_scores_gemma":[0.99934095,0.00007661627,0.00028650125,0.000021898237,0.0000027282038,0.0000028857073,0.00012634609,0.000005274381,0.00013686073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999356,0.0000024523536,0.0000028042143,0.000018211462,0.00001631934,0.000024553174],"domain_scores_gemma":[0.99987435,0.000012268572,0.00005678598,0.000009853037,0.00001384369,0.000032958047],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013296647,0.00027667443,0.00025445147,0.000554584,0.0003731629,0.00060346175,0.00042508694,0.00028241644,0.001139395],"category_scores_gemma":[0.00033371497,0.000226933,0.00027921412,0.00034417826,0.0003532725,0.00034615392,0.0003852788,0.00023142545,0.00017376934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028815723,0.000104142324,0.49149612,0.00013861398,0.00016857169,0.0011610978,0.00027657716,0.018570209,0.47153306,0.0033723183,0.00048422138,0.012406903],"study_design_scores_gemma":[0.000046904246,0.00007413234,0.9546237,0.00001677318,0.000039902287,0.00027938696,0.000115392526,0.026243052,0.016059214,0.0013299235,0.0011539512,0.000017673887],"about_ca_topic_score_codex":0.029593527,"about_ca_topic_score_gemma":0.018800147,"teacher_disagreement_score":0.029593527,"about_ca_system_score_codex":0.0015485045,"about_ca_system_score_gemma":0.00038245923,"threshold_uncertainty_score":0.05884254},"labels":[],"label_agreement":null},{"id":"W3175238256","doi":"10.3847/1538-4357/ac0cf3","title":"ZFIRE: The Beginning of the End for Massive Galaxies at z ∼ 2 and Why Environment Matters","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Galaxy; Redshift; Star formation; Field (mathematics); Galaxy formation and evolution; Stellar mass; Luminous infrared galaxy; Spectral energy distribution","score_opus":0.0061408299632310336,"score_gpt":0.18810371137114976,"score_spread":0.18196288140791872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3175238256","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95259005,0.0006002666,0.019308798,0.0024189684,0.000060903745,0.000017812894,0.0049069347,0.004245498,0.015850825],"genre_scores_gemma":[0.9861653,0.00012095867,0.0073257056,0.0003554451,0.000019600819,0.000011118963,0.0033766236,0.0009053699,0.0017199229],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983275,0.0000315525,0.0000034423877,0.000058660535,0.0000322198,0.000041325737],"domain_scores_gemma":[0.9994281,0.00019008016,0.0000803941,0.0001007845,0.00006253884,0.00013803881],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007968932,0.00031164067,0.00039434002,0.00030258947,0.0005950848,0.00135116,0.00065097155,0.00054677343,0.0047148974],"category_scores_gemma":[0.0027742102,0.00031572694,0.00050717103,0.0003337258,0.00040077665,0.0016276544,0.00088195316,0.0010876211,0.0009356051],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001506249,0.00014892337,0.6758199,0.0002603421,0.0003262584,0.0011235779,0.002760764,0.10953726,0.022577623,0.06947773,0.05113116,0.06533024],"study_design_scores_gemma":[0.0002860474,0.00020917042,0.5330284,0.00014890016,0.0001680874,0.0006069517,0.0011493725,0.34445584,0.016387668,0.057709802,0.045661215,0.00018849887],"about_ca_topic_score_codex":0.015345247,"about_ca_topic_score_gemma":0.012476361,"teacher_disagreement_score":0.015345247,"about_ca_system_score_codex":0.00046985375,"about_ca_system_score_gemma":0.00027233784,"threshold_uncertainty_score":0.030511856},"labels":[],"label_agreement":null},{"id":"W3175506586","doi":"10.3847/1538-4357/ac0cf2","title":"HAWC+/SOFIA Polarimetry in L1688: Relative Orientation of Magnetic Field and Elongated Cloud Structure","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Ophiuchus; Molecular cloud; Magnetic field; Planck; Orientation (vector space); Polarimetry; Perpendicular","score_opus":0.004834609494273806,"score_gpt":0.22996346819985133,"score_spread":0.22512885870557753,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3175506586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99933213,0.000010533925,0.000060674778,0.000006194052,9.268577e-7,0.000001493158,0.00015554724,0.000010402091,0.00042204713],"genre_scores_gemma":[0.99956447,0.0000063541715,0.00015512842,0.0000037370921,0.0000013930282,0.0000013586737,0.00018916532,0.000004319734,0.00007411559],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999336,0.0000068637464,0.000002750028,0.000021511616,0.000014623637,0.000020643216],"domain_scores_gemma":[0.99983454,0.000015119604,0.00006657901,0.000019700226,0.000027597398,0.000036281082],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012819411,0.00016711694,0.00020788588,0.0005141378,0.00031721863,0.00030436972,0.00015889085,0.00010237558,0.00086258195],"category_scores_gemma":[0.00024084028,0.000093903094,0.000109975204,0.0003480351,0.0002619412,0.00014027704,0.00040143376,0.0001344868,0.00021993787],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038223778,0.00003532141,0.8978154,0.00003518941,0.000050255207,0.00052321027,0.0004358383,0.0019037707,0.08487325,0.00025819955,0.00063080725,0.013056516],"study_design_scores_gemma":[0.0000070120163,0.00002319218,0.995626,0.000003249922,0.0000056935733,0.000100116915,0.00013119432,0.0013418541,0.0021897503,0.000038902464,0.0005284112,0.0000046428795],"about_ca_topic_score_codex":0.010146103,"about_ca_topic_score_gemma":0.015198759,"teacher_disagreement_score":0.010146103,"about_ca_system_score_codex":0.00039851002,"about_ca_system_score_gemma":0.0001342718,"threshold_uncertainty_score":0.020174086},"labels":[],"label_agreement":null},{"id":"W3175825478","doi":"10.3847/1538-4357/ac26b6","title":"Constraining Cosmic Microwave Background Temperature Evolution With Sunyaev–Zel’Dovich Galaxy Clusters from the Atacama Cosmology Telescope","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; National Research Foundation; National Aeronautics and Space Administration","keywords":"Cosmic microwave background; Galaxy cluster; Black-body radiation; Cosmology; Redshift; Cosmic background radiation; Observational cosmology; Galaxy; Background radiation","score_opus":0.00862217020251541,"score_gpt":0.209171729712776,"score_spread":0.2005495595102606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3175825478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99603075,0.00010130829,0.0006773479,0.0000551579,0.000007537238,0.000008360309,0.0015546172,0.000052766773,0.001512138],"genre_scores_gemma":[0.9955415,0.000032759726,0.00074536045,0.000022417447,0.000014727936,0.000009336111,0.0033010133,0.000034665765,0.00029825378],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99961394,0.000057450525,0.000013947276,0.00014824749,0.00008678387,0.00007970208],"domain_scores_gemma":[0.99824214,0.00023401808,0.0004319977,0.00042485265,0.00018575897,0.00048131784],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007710904,0.00030492304,0.0004283256,0.0013842672,0.00061691366,0.00086126867,0.000511369,0.00021508001,0.0014659348],"category_scores_gemma":[0.001462761,0.0003332324,0.0004182804,0.0012388027,0.00031545133,0.00024957303,0.0009217247,0.0003444858,0.0004208648],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002503637,0.00004167272,0.9825174,0.000020115225,0.00019768695,0.00009114607,0.00024260968,0.003855979,0.0049072695,0.0006216689,0.0020427068,0.0052114935],"study_design_scores_gemma":[0.000016398131,0.000009981269,0.99448663,0.000003846269,0.000021847154,0.000012872869,0.000052475367,0.0035481697,0.00058311695,0.00008142843,0.0011771357,0.0000061034293],"about_ca_topic_score_codex":0.056678835,"about_ca_topic_score_gemma":0.059961494,"teacher_disagreement_score":0.056678835,"about_ca_system_score_codex":0.0011844496,"about_ca_system_score_gemma":0.0004051261,"threshold_uncertainty_score":0.11269784},"labels":[],"label_agreement":null},{"id":"W3177653350","doi":"10.3847/1538-4357/ac3cb6","title":"Search for High-energy Neutrinos from Ultraluminous Infrared Galaxies with IceCube","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Office of Polar Programs; Santen; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Astrophysics; Neutrino","score_opus":0.0088343156796083,"score_gpt":0.20683875437666419,"score_spread":0.1980044386970559,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3177653350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9682675,0.0002096236,0.0038617128,0.00011395667,0.000028161689,0.000087585184,0.018217945,0.00077532075,0.008438156],"genre_scores_gemma":[0.9156616,0.00022081849,0.019997086,0.00014904779,0.000040672276,0.00014802109,0.061928265,0.0001416951,0.001712713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997303,0.00004599089,0.00001562906,0.00007955537,0.00007127367,0.000057324705],"domain_scores_gemma":[0.99920326,0.00019214937,0.00020748739,0.00015269178,0.00010758444,0.00013689775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007753504,0.000349356,0.0003610061,0.0012751659,0.00035868175,0.0007642662,0.0004526029,0.00021491396,0.0016436668],"category_scores_gemma":[0.00079536793,0.0002069007,0.0004872474,0.0018814148,0.00017693668,0.00022626236,0.0005644218,0.00024082672,0.00050569413],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018090198,0.000283189,0.8899967,0.00011039023,0.00061258586,0.00049761694,0.00056113314,0.008492594,0.03851872,0.0016800219,0.01593607,0.041502014],"study_design_scores_gemma":[0.00015224799,0.00031901666,0.8754532,0.000041052088,0.0002760043,0.0003656491,0.0006163368,0.0319529,0.038725417,0.0013029237,0.050761927,0.000033290107],"about_ca_topic_score_codex":0.0075001735,"about_ca_topic_score_gemma":0.011053292,"teacher_disagreement_score":0.0075001735,"about_ca_system_score_codex":0.0004057455,"about_ca_system_score_gemma":0.00039241902,"threshold_uncertainty_score":0.0149130225},"labels":[],"label_agreement":null},{"id":"W3177894565","doi":"10.3847/1538-4357/ac2610","title":"Binary Black Hole Formation with Detailed Modeling: Stable Mass Transfer Leads to Lower Merger Rates","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Quest High Performance Computing; Fonds Wetenschappelijk Onderzoek; Canadian Institute for Advanced Research; Northwestern University; Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Common envelope; Physics; Black hole (networking); Astrophysics; Population; Binary black hole; Metallicity; Mass transfer; Binary number; COSMIC cancer database; Solar mass; Gravitational wave; Stars; White dwarf; Mechanics","score_opus":0.020589837043092255,"score_gpt":0.29976995645310606,"score_spread":0.2791801194100138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3177894565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889026,0.00012634932,0.007050191,0.00010370588,0.000012962574,0.000013994781,0.00035337545,0.00020150631,0.0032351257],"genre_scores_gemma":[0.9987086,0.000029501554,0.0009268021,0.000017444007,0.0000035590776,0.0000064051915,0.00009487721,0.000026023738,0.00018662156],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998766,0.000032947242,0.0000071328473,0.000036770984,0.000022217579,0.000024327279],"domain_scores_gemma":[0.9992393,0.00036129818,0.00015759657,0.00011353745,0.000058057867,0.00007024025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038369757,0.000503678,0.00047150237,0.0003934366,0.0002525922,0.0009622263,0.0006750183,0.0005143726,0.0021365718],"category_scores_gemma":[0.001785455,0.00021195527,0.00056270376,0.00028418854,0.0003762116,0.00073191687,0.0005647105,0.00035830613,0.00021769009],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001415052,0.00008700971,0.025851203,0.000057983292,0.00008891039,0.00011689024,0.00006385515,0.95613265,0.008955207,0.0046534333,0.00035704864,0.0034941568],"study_design_scores_gemma":[0.000027250308,0.00005545026,0.0067865904,0.0000055820838,0.000033511096,0.000034868233,0.000022564944,0.98707134,0.003922316,0.001605268,0.00042287324,0.0000124065955],"about_ca_topic_score_codex":0.0068097757,"about_ca_topic_score_gemma":0.0025130373,"teacher_disagreement_score":0.0068097757,"about_ca_system_score_codex":0.0008461399,"about_ca_system_score_gemma":0.00038417138,"threshold_uncertainty_score":0.013540268},"labels":[],"label_agreement":null},{"id":"W3179074945","doi":"10.3847/1538-4357/ac47f7","title":"Snails across Scales: Local and Global Phase-mixing Structures as Probes of the Past and Future Milky Way","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Ministry of Education, Culture, Sports, Science and Technology; European Commission; York University; Flatiron Health; Aspen Center for Physics; Simons Foundation; European Research Council; National Science Foundation","keywords":"Physics; Milky Way; Astrophysics; Stars; Spiral galaxy; Disc; Galaxy formation and evolution; Galaxy","score_opus":0.00639607646583257,"score_gpt":0.24507526300744678,"score_spread":0.2386791865416142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3179074945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99850863,0.000023872048,0.00076634815,0.00007605457,0.000002448868,0.000003642016,0.000024652152,0.000019371908,0.0005749763],"genre_scores_gemma":[0.9996253,0.000011229331,0.00026002963,0.000007036377,0.0000013203787,0.0000021733188,0.00001821425,0.000006447934,0.00006811717],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99995136,0.000014113565,0.0000024899025,0.0000129557575,0.0000064205233,0.000012628849],"domain_scores_gemma":[0.99971634,0.00008424799,0.0000619863,0.000028970633,0.000017086464,0.00009136751],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031152242,0.00015117349,0.00028237712,0.00029601975,0.00034380765,0.0008312898,0.00037711282,0.00038132662,0.0011695671],"category_scores_gemma":[0.0013063082,0.00021188354,0.0003121893,0.0002349467,0.0006240425,0.0007741506,0.00081909145,0.00043758837,0.00006027685],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006369747,0.00031485115,0.2477182,0.00008946495,0.0003604554,0.00075610843,0.0015962082,0.6952869,0.024378289,0.01830228,0.001108572,0.009451735],"study_design_scores_gemma":[0.00010378783,0.00025412618,0.100434355,0.000015606593,0.00005354649,0.00007556416,0.00079924014,0.88908833,0.0019051675,0.0064580315,0.0007707111,0.000041498406],"about_ca_topic_score_codex":0.0060871383,"about_ca_topic_score_gemma":0.0045241904,"teacher_disagreement_score":0.0060871383,"about_ca_system_score_codex":0.00053786667,"about_ca_system_score_gemma":0.0002832726,"threshold_uncertainty_score":0.012103379},"labels":[],"label_agreement":null},{"id":"W3179302479","doi":"10.3847/1538-4357/ac3330","title":"Late-time Evolution and Modeling of the Off-axis Gamma-Ray Burst Candidate FIRST J141918.9+394036","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; York University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of Toronto; Associated Universities; Canada Research Chairs; California Institute of Technology; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Gamma-ray burst; Physics; Computer science; Astrophysics","score_opus":0.00806313221652676,"score_gpt":0.2044530838033333,"score_spread":0.19638995158680653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3179302479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982786,0.0000491274,0.0007886894,0.00003930619,0.0000042683337,0.00000571962,0.00022669231,0.000042015563,0.00056567485],"genre_scores_gemma":[0.9987835,0.000020457743,0.0004542915,0.000007451551,0.0000033463073,0.0000047888634,0.0004195057,0.000016152782,0.00029056065],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999306,0.00000628809,0.0000030760891,0.000020709605,0.000012276718,0.00002697353],"domain_scores_gemma":[0.99974996,0.00003351797,0.00008187798,0.000020503587,0.00003582699,0.00007827111],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025650117,0.00034716638,0.00029529113,0.00069182465,0.00039173095,0.0007368227,0.00082231854,0.0005146121,0.0013506422],"category_scores_gemma":[0.00044988396,0.00023353698,0.00051641156,0.00041042562,0.0001891167,0.00027572695,0.0003363454,0.00026352232,0.00036938707],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037418355,0.00019988799,0.85118574,0.000041454125,0.00013610379,0.0014810938,0.00019034884,0.10482168,0.030340143,0.0014047484,0.0006890393,0.009135573],"study_design_scores_gemma":[0.00004819751,0.00015060567,0.5233553,0.000015930651,0.00009155522,0.00038958288,0.0002376103,0.4701646,0.0030510307,0.0006467414,0.0018124832,0.00003637442],"about_ca_topic_score_codex":0.020674132,"about_ca_topic_score_gemma":0.017216818,"teacher_disagreement_score":0.020674132,"about_ca_system_score_codex":0.0009947395,"about_ca_system_score_gemma":0.00041342585,"threshold_uncertainty_score":0.041107595},"labels":[],"label_agreement":null},{"id":"W3180036870","doi":"10.3847/1538-4357/ac1115","title":"On the Use of Field RR Lyrae As Galactic Probes: IV. New Insights Into and Around the Oosterhoff Dichotomy*","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; Science and Technology Facilities Council; National Development and Reform Commission; Los Alamos National Laboratory; National Astronomical Observatory of Japan; Chinese Academy of Sciences; Istituto Nazionale di Astrofisica; University of Pittsburgh; Johns Hopkins University; National Astronomical Observatories, Chinese Academy of Sciences; Max-Planck-Gesellschaft; Carnegie Institution of Washington; Deutsche Forschungsgemeinschaft; New Mexico State University; Agenzia Spaziale Italiana; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; U.S. Department of Energy","keywords":"RR Lyrae variable; Metallicity; Astrophysics; Physics; Amplitude; Population; Metal; Spectral line; Analytical Chemistry (journal); Chemistry; Galaxy; Astronomy; Optics","score_opus":0.02062951023405747,"score_gpt":0.23431300260510687,"score_spread":0.2136834923710494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3180036870","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94911665,0.02333704,0.009771053,0.0021142971,0.000056581335,0.000016134261,0.0003669241,0.00008175281,0.015139526],"genre_scores_gemma":[0.9917911,0.0031672285,0.0034940268,0.00038247815,0.00017609404,0.000008829178,0.00016667988,0.000024122548,0.0007895187],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994331,0.00023930149,0.000023038552,0.00018522884,0.00006559168,0.00005365919],"domain_scores_gemma":[0.99731344,0.0016182049,0.00037079587,0.0003864902,0.00018166452,0.00012941923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0035738288,0.00039062175,0.00042311146,0.0019287531,0.00027878507,0.0026802935,0.000595606,0.0003677301,0.0013862592],"category_scores_gemma":[0.0033265469,0.00013117782,0.00015026392,0.0011432153,0.0016203074,0.0038836352,0.00091228075,0.00044019695,0.00026429427],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056512683,0.00010377256,0.58274466,0.00034582146,0.00016404953,0.00026260858,0.0027312248,0.0010192724,0.014719853,0.029821545,0.0018824908,0.36563966],"study_design_scores_gemma":[0.000030177247,0.00028594973,0.9144613,0.00027638837,0.00009825249,0.00036670375,0.004752474,0.004811171,0.0038292685,0.03730056,0.03371478,0.00007296214],"about_ca_topic_score_codex":0.002012583,"about_ca_topic_score_gemma":0.0024917237,"teacher_disagreement_score":0.0035738288,"about_ca_system_score_codex":0.0004158062,"about_ca_system_score_gemma":0.00014380513,"threshold_uncertainty_score":0.018900454},"labels":[],"label_agreement":null},{"id":"W3180268056","doi":"10.3847/1538-4357/ac7043","title":"Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey. I. Evidence for Thermal Energy Anisotropy Using Oriented Stacking","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"SLAC National Accelerator Laboratory; Integrated Electronics Engineering Center, Binghamton University; European Regional Development Fund; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of Illinois at Urbana-Champaign; European Research Council; National Institute of Standards and Technology; Institut de Física d'Altes Energies; Connaught Fund; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Generalitat de Catalunya; Office of Science; University of Edinburgh; University of Sussex; University of Nottingham; University of Toronto; Ohio State University; National Research Foundation; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration; University College London; University of Cambridge; National Energy Research Scientific Computing Center; University of Portsmouth; University of Chicago; Ministério da Ciência, Tecnologia e Inovação; Lawrence Berkeley National Laboratory; Financiadora de Estudos e Projetos; University of Pennsylvania; High Energy Physics; Deutsche Forschungsgemeinschaft; Argonne National Laboratory; Centres de Recerca de Catalunya; Ministerio de Ciencia e Innovación; European Commission; U.S. Department of Energy; Princeton University; University of Michigan; Fermilab; National Science Foundation","keywords":"Physics; Cosmic microwave background; Galaxy cluster; Astrophysics; Dark energy; Cosmology; Galaxy; Astronomy; South Pole Telescope; Large Synoptic Survey Telescope; Telescope; Anisotropy; Optics","score_opus":0.02336722086131838,"score_gpt":0.24483561114159536,"score_spread":0.22146839028027698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3180268056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99548846,0.000072338815,0.0015714903,0.00010029477,0.000008111022,0.000012199554,0.0009601519,0.00017023546,0.0016167711],"genre_scores_gemma":[0.9958556,0.000028892022,0.0027805849,0.000023981582,0.0000120607665,0.000008043234,0.0010653528,0.0000631132,0.0001623196],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997881,0.00006220115,0.000008674019,0.000060827224,0.000051070307,0.000029131359],"domain_scores_gemma":[0.9991352,0.00018608249,0.0002595504,0.00015097945,0.0000849876,0.00018323651],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071257126,0.00033682192,0.00033908902,0.0006877722,0.00039709004,0.0006017639,0.00055069535,0.00027840893,0.001220636],"category_scores_gemma":[0.0012899995,0.0002883031,0.0005254003,0.0009234107,0.00035498146,0.0003682321,0.0006476883,0.00041655582,0.00020680013],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000738466,0.00018470596,0.7973115,0.000090975955,0.00092365313,0.00041770228,0.0003833558,0.15793139,0.018013585,0.0049747084,0.0046704635,0.014359682],"study_design_scores_gemma":[0.00009024963,0.00004997623,0.55701613,0.000013830123,0.0000742784,0.000072318646,0.00011946674,0.4372126,0.0025368144,0.0016012485,0.0011811776,0.000031993543],"about_ca_topic_score_codex":0.03260849,"about_ca_topic_score_gemma":0.029135194,"teacher_disagreement_score":0.03260849,"about_ca_system_score_codex":0.0005750977,"about_ca_system_score_gemma":0.00027961,"threshold_uncertainty_score":0.06483734},"labels":[],"label_agreement":null},{"id":"W3180827751","doi":"10.3847/1538-4357/ac1106","title":"ALMA Observations of Lyα Blob 1: Multiple Major Mergers and Widely Distributed Interstellar Media","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Japan Society for the Promotion of Science; Science and Technology Facilities Council; Deutsche Forschungsgemeinschaft","keywords":"Physics; Astrophysics; Star formation; Galaxy; Millimeter; Interstellar medium; Submillimeter Array; Astronomy; Infrared; H-alpha; Emission spectrum; Spectral line","score_opus":0.013730910942588376,"score_gpt":0.2073594854351428,"score_spread":0.1936285744925544,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3180827751","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989526,0.00005575443,0.000074297954,0.000010662689,0.0000011813121,0.0000029319792,0.000181567,0.000024473775,0.00069641916],"genre_scores_gemma":[0.9993498,0.000014932919,0.00012527242,0.000008223887,0.0000032827995,0.0000024123644,0.00023891055,0.000002726618,0.00025431314],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999553,0.0000027976982,0.0000016437724,0.000011070853,0.00001483498,0.000014399634],"domain_scores_gemma":[0.9998317,0.000008250986,0.000049929844,0.000009229058,0.000026642434,0.00007418879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007177959,0.00017220566,0.00016170547,0.0006601979,0.00037585988,0.00028521483,0.00020678535,0.00018952251,0.0011782354],"category_scores_gemma":[0.000115535964,0.00010751645,0.00011044907,0.00034400928,0.00013981141,0.0001540637,0.00037811272,0.00017766313,0.00038206382],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026535694,0.00006685731,0.7981775,0.000031261785,0.000062574654,0.0015194321,0.0005242124,0.00033314814,0.19081573,0.000119383185,0.0007065069,0.0073781507],"study_design_scores_gemma":[0.000005629544,0.00004465897,0.9960001,0.0000018158919,0.000008109258,0.0002826968,0.000101728736,0.00033108052,0.0026043311,0.000014165567,0.00060290477,0.0000026660616],"about_ca_topic_score_codex":0.005335148,"about_ca_topic_score_gemma":0.011167257,"teacher_disagreement_score":0.005335148,"about_ca_system_score_codex":0.0003059437,"about_ca_system_score_gemma":0.00007552779,"threshold_uncertainty_score":0.010608196},"labels":[],"label_agreement":null},{"id":"W3181990790","doi":"10.3847/1538-4357/ac1583","title":"A Deep Search for Five Molecules in the 49 Ceti Debris Disk","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Debris; Photodissociation; Astrochemistry; Stars; Solar System; Millimeter; Astronomy; Protoplanetary disk; Astrobiology; Interstellar medium; Chemistry; Galaxy","score_opus":0.017542422566926768,"score_gpt":0.2778529325143004,"score_spread":0.2603105099473736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3181990790","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983315,0.00016381417,0.00032967987,0.000030376761,0.0000018751855,0.0000059688714,0.00019158101,0.000014280885,0.0009308941],"genre_scores_gemma":[0.9984668,0.00007475332,0.00081099547,0.00002180445,0.0000047344365,0.0000034026737,0.000359951,0.0000030838696,0.00025437426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994695,0.000002702043,0.0000017546247,0.000018075356,0.000012152012,0.000018270815],"domain_scores_gemma":[0.9998292,0.000020038042,0.000044450233,0.000016707385,0.000018896142,0.00007063656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009380912,0.00016959905,0.00021855399,0.0007033984,0.00042059645,0.00041696263,0.0002572857,0.00027426606,0.0011910207],"category_scores_gemma":[0.00015367518,0.00013827663,0.00013608538,0.000342084,0.00016184831,0.00024601625,0.00053315336,0.00021307946,0.00026295712],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033226176,0.00013879796,0.49906364,0.00007571205,0.00005591624,0.00067292474,0.00056516106,0.00069146784,0.46737155,0.00034596678,0.00033513966,0.03035139],"study_design_scores_gemma":[0.00002234308,0.00026960092,0.9565739,0.000015053688,0.000043885528,0.0006533798,0.0005658509,0.0035762824,0.0338005,0.000240893,0.0042273747,0.000010909125],"about_ca_topic_score_codex":0.0010429408,"about_ca_topic_score_gemma":0.0016747542,"teacher_disagreement_score":0.0011910207,"about_ca_system_score_codex":0.00021321684,"about_ca_system_score_gemma":0.00012495327,"threshold_uncertainty_score":0.003984332},"labels":[],"label_agreement":null},{"id":"W3182158366","doi":"10.3847/1538-4357/ac126a","title":"Polarization Pipeline for Fast Radio Bursts Detected by CHIME/FRB","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Advanced Frequency and Time Standards","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; McGill University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Fast radio burst; Polarization (electrochemistry); Linear polarization; Faraday effect; Astrophysics; Optics; Magnetic field; Laser","score_opus":0.007237468516699851,"score_gpt":0.2499460439197308,"score_spread":0.24270857540303095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3182158366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90466493,0.00015516426,0.07126123,0.0003745628,0.000042576965,0.00019905291,0.0071380935,0.0088770995,0.0072871665],"genre_scores_gemma":[0.9085101,0.0000929636,0.08067742,0.00008761652,0.00003638008,0.000093140465,0.008638894,0.0005333482,0.001330192],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997613,0.00001912435,0.000006967695,0.000041730567,0.000100726116,0.000070289134],"domain_scores_gemma":[0.9995277,0.00007554232,0.00007144882,0.00006817115,0.00018189638,0.00007511237],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057489984,0.00050013105,0.00033808948,0.0019379448,0.00054744876,0.00061721826,0.0005642841,0.00036125514,0.0032829675],"category_scores_gemma":[0.0008480699,0.0003350124,0.00041225128,0.0012786777,0.00018899576,0.0003457186,0.0006673695,0.00049480906,0.0008977293],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015911118,0.00025670842,0.17872998,0.0002091444,0.00023611139,0.00073859823,0.0006330056,0.020871654,0.54615176,0.0016663772,0.007306951,0.24160853],"study_design_scores_gemma":[0.00015669476,0.00039533482,0.54401773,0.000042092342,0.00014680158,0.0005046993,0.00030141915,0.25492853,0.18392637,0.0015905001,0.013798639,0.00019112429],"about_ca_topic_score_codex":0.01401294,"about_ca_topic_score_gemma":0.02616058,"teacher_disagreement_score":0.01401294,"about_ca_system_score_codex":0.0006891372,"about_ca_system_score_gemma":0.0009523773,"threshold_uncertainty_score":0.027862728},"labels":[],"label_agreement":null},{"id":"W3182657995","doi":"10.3847/1538-4357/ac1074","title":"On the Use of Field RR Lyrae as Galactic Probes. V. Optical and Radial Velocity Curve Templates","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"U.S. Department of Energy; U.S. Naval Observatory; Japan Society for the Promotion of Science; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; Deutsche Forschungsgemeinschaft; New Mexico State University; University of Portsmouth; Science and Technology Facilities Council; Universität Basel; Istituto Nazionale di Astrofisica; University of Pittsburgh; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; Princeton University; Johns Hopkins University; Ohio State University; Agenzia Spaziale Italiana; Fermilab; Case Western Reserve University; National Science Foundation; Drexel University; National Aeronautics and Space Administration","keywords":"RR Lyrae variable; Astrophysics; Template; Field (mathematics); Physics; Radial velocity; Light curve; Astronomy; Galaxy; Materials science; Mathematics; Nanotechnology; Globular cluster; Pure mathematics","score_opus":0.023755938765682296,"score_gpt":0.23727215274272812,"score_spread":0.21351621397704582,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3182657995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8824685,0.00076391554,0.08429184,0.0001149226,0.000047976777,0.00018529808,0.012302376,0.004420241,0.0154048605],"genre_scores_gemma":[0.92694485,0.00013824164,0.0617878,0.000069524795,0.000033928012,0.00010126387,0.009378493,0.0003398402,0.0012061049],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987112,0.00040067005,0.00008553939,0.0004248456,0.00028061896,0.00009711221],"domain_scores_gemma":[0.994443,0.0009363944,0.0011859076,0.0022994925,0.0009334449,0.00020176615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024079608,0.00036247447,0.00025017292,0.0017944827,0.00023928272,0.0010640479,0.0007600526,0.00034945257,0.00144336],"category_scores_gemma":[0.0068728365,0.00023328261,0.00026088618,0.001370229,0.00019045382,0.0007474031,0.000618302,0.00023774021,0.0018806083],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028456867,0.00013212764,0.70492953,0.00011178792,0.0001242181,0.00009432602,0.0004132755,0.019107215,0.022152953,0.0032445823,0.0040255096,0.24537988],"study_design_scores_gemma":[0.000042270298,0.00015719362,0.9005642,0.00004873445,0.000056888497,0.00021886492,0.0002132136,0.049649138,0.020315904,0.0014705104,0.027205685,0.000057382378],"about_ca_topic_score_codex":0.0049734977,"about_ca_topic_score_gemma":0.0064739273,"teacher_disagreement_score":0.0049734977,"about_ca_system_score_codex":0.00041739715,"about_ca_system_score_gemma":0.00023173503,"threshold_uncertainty_score":0.012734711},"labels":[],"label_agreement":null},{"id":"W3183230540","doi":"10.3847/1538-4357/ac49e1","title":"Modeling Fast Radio Burst Dispersion and Scattering Properties in the First CHIME/FRB Catalog","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; Perimeter Institute; Canadian Institute for Theoretical Astrophysics; University of Waterloo; University of Toronto; University of British Columbia; McGill University","funders":"McGill Space Institute; National Defense Science and Engineering Graduate; Smithsonian Astrophysical Observatory; Fondation familiale Trottier; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; National Research Council Canada; University of Toronto; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Research Chairs; Industry Canada; Fonds de recherche du Québec – Nature et technologies; National Radio Astronomy Observatory; National Science Foundation; Compute Canada; McGill University; Associated Universities; University of British Columbia; U.S. Department of Defense; Canadian Institute for Advanced Research; Government of Canada","keywords":"Physics; Astrophysics; Scattering; Population; Galaxy; Milky Way; Fast radio burst; Interstellar medium; Pulsar; Velocity dispersion; Astronomy; Optics","score_opus":0.01596013341958718,"score_gpt":0.2627204286257355,"score_spread":0.24676029520614834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3183230540","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99559563,0.000044986835,0.0028101925,0.00005863821,0.0000029688906,0.000025675443,0.0005795787,0.0000863247,0.000795979],"genre_scores_gemma":[0.99499595,0.000030563948,0.0031385345,0.0000240879,0.0000035827445,0.000029739736,0.0014168983,0.000026680731,0.0003340578],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99976104,0.00006169753,0.0000059782283,0.00007749845,0.000043788674,0.000050107534],"domain_scores_gemma":[0.9981292,0.00096560724,0.00018590046,0.00026564836,0.0003047876,0.0001488742],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015738598,0.00037937588,0.00044425836,0.0008202376,0.0006633458,0.00079802016,0.0011294709,0.00076633587,0.001077711],"category_scores_gemma":[0.0036336381,0.00040906784,0.0006356758,0.0007591354,0.0005855313,0.0005706729,0.00045393608,0.0004867344,0.0001801123],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010285839,0.000072888775,0.08087938,0.000013865926,0.000076871285,0.00008206249,0.00010835049,0.9119635,0.0009619391,0.0017218336,0.00055531214,0.0034612243],"study_design_scores_gemma":[0.000042863485,0.000040944295,0.019685963,0.0000040141467,0.00001761098,0.00003227613,0.000041227227,0.9786395,0.0005382753,0.0005229661,0.00041997587,0.00001443069],"about_ca_topic_score_codex":0.17781886,"about_ca_topic_score_gemma":0.119023435,"teacher_disagreement_score":0.17781886,"about_ca_system_score_codex":0.0029821298,"about_ca_system_score_gemma":0.001237631,"threshold_uncertainty_score":0.35356766},"labels":[],"label_agreement":null},{"id":"W3183567758","doi":"10.3847/1538-4357/ac178b","title":"Weather on Other Worlds. VI. Optical Spectrophotometry of Luhman 16B Reveals Large-amplitude Variations in the Alkali Lines","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Université de Liège; Agencia Nacional de Investigación y Desarrollo; California Institute of Technology; National Aeronautics and Space Administration; Fonds De La Recherche Scientifique - FNRS; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Space Telescope Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Angstrom; Astrophysics; Wavelength; Amplitude; Spectrograph; Spectral line; Alkali metal; Physics; Flux (metallurgy); Analytical Chemistry (journal); Chemistry; Optics; Astronomy","score_opus":0.013540420039846034,"score_gpt":0.26014853084313694,"score_spread":0.2466081108032909,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3183567758","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4919081,0.005106332,0.0017707524,0.010408808,0.0038415017,0.00009943678,0.011340237,0.0006764383,0.47484845],"genre_scores_gemma":[0.80149156,0.0026542204,0.0018395307,0.0021986398,0.0007764099,0.000026775186,0.004546571,0.00020020142,0.18626603],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.0000127507,0.000010822122,0.000026175265,0.000033907832,0.000038497794],"domain_scores_gemma":[0.9996605,0.0000136049575,0.0000916447,0.00006619334,0.00006594572,0.000102174585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016477938,0.00017478233,0.00018091439,0.0004289087,0.0009857997,0.0014503739,0.00016538889,0.00029940903,0.032481622],"category_scores_gemma":[0.00038396087,0.00007095665,0.00014883195,0.00056685705,0.00032616142,0.0010005945,0.0010494051,0.00062582514,0.008162963],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007835452,0.0002471117,0.33152232,0.00042566963,0.00031570878,0.0025485556,0.0038708812,0.0009885428,0.033965193,0.019592166,0.21795127,0.3877891],"study_design_scores_gemma":[0.0000180326,0.00007197922,0.1916833,0.00013287045,0.000028386366,0.0005121618,0.0032760072,0.00026313117,0.0017779905,0.0016052843,0.8005992,0.00003158693],"about_ca_topic_score_codex":0.0061164526,"about_ca_topic_score_gemma":0.014204333,"teacher_disagreement_score":0.032481622,"about_ca_system_score_codex":0.00036209193,"about_ca_system_score_gemma":0.000308481,"threshold_uncertainty_score":0.10866183},"labels":[],"label_agreement":null},{"id":"W3184971005","doi":"10.3847/1538-4357/ac540d","title":"On the Use of CHIME to Detect Long-duration Radio Transients from Neutron Star Mergers","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia","funders":"Japan Society for the Promotion of Science","keywords":"Afterglow; Gravitational wave; Neutron star; Physics; Gamma-ray burst; Astrophysics; Binary number; Jet (fluid); Kilonova; LIGO; Star (game theory); Astronomy; Mathematics","score_opus":0.018686999311346396,"score_gpt":0.21756397340402034,"score_spread":0.19887697409267394,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3184971005","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9833108,0.00028339837,0.011799367,0.00011308191,0.0000073929828,0.00008185016,0.0010282722,0.0004758225,0.0028999879],"genre_scores_gemma":[0.9885014,0.00003799591,0.010683448,0.000024012495,0.0000018922264,0.000010334956,0.00048472008,0.000014217967,0.00024194195],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997044,0.00005730327,0.000006974465,0.00007605479,0.00010387361,0.000051192612],"domain_scores_gemma":[0.9990625,0.00047541386,0.000113977294,0.0000903667,0.00014681148,0.00011091321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009766741,0.00041005015,0.00028397513,0.0013891053,0.00037978205,0.00044947607,0.000385545,0.00031623305,0.0008571792],"category_scores_gemma":[0.0023059235,0.00017100334,0.00022637198,0.0005352385,0.00031564088,0.00030492333,0.00044120412,0.0001610604,0.00013572162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013707938,0.00013360972,0.7829854,0.00013231495,0.0001962172,0.00036151978,0.00012285741,0.04562747,0.087400734,0.0015087521,0.0009689692,0.07919135],"study_design_scores_gemma":[0.00007976737,0.00023298095,0.7880274,0.00002173943,0.000079097874,0.00031848394,0.00016397574,0.1741007,0.034402914,0.0006303139,0.0018619156,0.000080574595],"about_ca_topic_score_codex":0.057495177,"about_ca_topic_score_gemma":0.109681465,"teacher_disagreement_score":0.057495177,"about_ca_system_score_codex":0.0009807859,"about_ca_system_score_gemma":0.00055534125,"threshold_uncertainty_score":0.11432105},"labels":[],"label_agreement":null},{"id":"W3185032300","doi":"10.3847/1538-4357/ac2e93","title":"Measuring the Mass of the Large Magellanic Cloud with Stellar Streams Observed by S <sup>5</sup>","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":114,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"SLAC National Accelerator Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Lawrence Berkeley National Laboratory; National Science Foundation; Fermilab; Institut de Física d'Altes Energies; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; University of Portsmouth; University of Chicago; Ohio State University; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; University of Sussex; Ministério da Ciência, Tecnologia e Inovação; University College London; National Aeronautics and Space Administration; Science and Technology Facilities Council; European Space Agency; Argonne National Laboratory; U.S. Department of Energy","keywords":"Physics; Large Magellanic Cloud; Astrophysics; Astronomy; STREAMS; Young stellar object; Stellar evolution; Stellar mass; Stars; Star formation","score_opus":0.015662392699407973,"score_gpt":0.1960669984132847,"score_spread":0.18040460571387673,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3185032300","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98940885,0.00007322305,0.002052177,0.00007241845,0.000011186088,0.000013954328,0.002878822,0.00038669203,0.0051026368],"genre_scores_gemma":[0.9952246,0.000021319152,0.0014527022,0.000030488663,0.000009251292,0.0000050038416,0.00273948,0.000036021236,0.000481179],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999212,0.000009471924,0.0000046604064,0.000021933029,0.000027101038,0.000015670135],"domain_scores_gemma":[0.99960333,0.000054836244,0.00011917256,0.000051724084,0.00007661403,0.00009437563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030103995,0.00019113638,0.00013607707,0.000549465,0.00017641748,0.00035557183,0.00021845668,0.00019158833,0.0027501318],"category_scores_gemma":[0.00063235924,0.00008645702,0.00023460355,0.00042828437,0.00011170633,0.00027163333,0.0002594752,0.000109243774,0.0010790378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010086532,0.000011112441,0.9788425,0.000011159349,0.000038931128,0.000045404282,0.000060584123,0.0018358633,0.0064192885,0.00022851807,0.0019062824,0.010499453],"study_design_scores_gemma":[0.000008201982,0.00004003903,0.97777486,0.000007730096,0.000033856857,0.000095923235,0.00011703546,0.012921836,0.0040628584,0.00021292562,0.004718343,0.0000064656024],"about_ca_topic_score_codex":0.007653566,"about_ca_topic_score_gemma":0.016127454,"teacher_disagreement_score":0.007653566,"about_ca_system_score_codex":0.00035308077,"about_ca_system_score_gemma":0.00012967002,"threshold_uncertainty_score":0.0152180195},"labels":[],"label_agreement":null},{"id":"W3186474699","doi":"10.3847/1538-4357/ac1679","title":"The JCMT Transient Survey: Four-year Summary of Monitoring the Submillimeter Variability of Protostars","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Dalhousie University; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Protostar; Physics; Submillimeter Array; Brightness; Accretion (finance); Amplitude; Astronomy; Star formation; Stars; Optics","score_opus":0.026268844560457763,"score_gpt":0.2587451282386139,"score_spread":0.23247628367815615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3186474699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9858073,0.00033167112,0.0008574104,0.00006555215,0.000011683366,0.000087646564,0.011208578,0.00024165119,0.0013885585],"genre_scores_gemma":[0.97748727,0.00020811215,0.0019111319,0.00007093833,0.00006797317,0.00008070673,0.019386686,0.00008173787,0.00070540875],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99930274,0.000074365045,0.00006771544,0.0001574341,0.000249887,0.00014783192],"domain_scores_gemma":[0.99345255,0.00044481215,0.002306841,0.00081748277,0.0014262483,0.0015520687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010696668,0.0003803654,0.00052406656,0.004523974,0.0006694117,0.00082382327,0.00065463706,0.00040760462,0.0010374029],"category_scores_gemma":[0.0023265537,0.00026336208,0.0004169676,0.0030593507,0.00032330517,0.00051516475,0.0010768432,0.00028010627,0.00057521695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011264476,0.000042709322,0.9848994,0.000038357626,0.000079571524,0.000159228,0.0001828806,0.00026601207,0.0052101864,0.000028363525,0.0014304994,0.0075500985],"study_design_scores_gemma":[0.0000031820318,0.000026283227,0.9985123,0.0000026963348,0.000014765393,0.00008370527,0.000026725736,0.000274307,0.00036680783,0.000003942881,0.00068245555,0.000002861144],"about_ca_topic_score_codex":0.021128422,"about_ca_topic_score_gemma":0.032669917,"teacher_disagreement_score":0.021128422,"about_ca_system_score_codex":0.00082667655,"about_ca_system_score_gemma":0.0006668453,"threshold_uncertainty_score":0.042010844},"labels":[],"label_agreement":null},{"id":"W3188976647","doi":"10.3847/1538-4357/ac1bb9","title":"A Core Mass Function Indistinguishable from the Salpeter Stellar Initial Mass Function Using 1000 au Resolution ALMA Observations","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Scientific Research and Discoveries","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Initial mass function; Flattening; Flux (metallurgy); Power law; Function (biology); Millimeter; Galaxy; Star formation; Astronomy; Statistics; Mathematics; Chemistry","score_opus":0.10888560582600511,"score_gpt":0.3108852613912031,"score_spread":0.201999655565198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3188976647","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9851062,0.0002527609,0.008809854,0.000058145153,0.000013694507,0.0000138825735,0.0010216745,0.0005322153,0.004191505],"genre_scores_gemma":[0.99397117,0.000033145338,0.0042912364,0.000026659101,0.000009131778,0.000008485453,0.0012333711,0.00007164181,0.00035512212],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998708,0.000010436502,0.0000049322334,0.000039036106,0.000040203257,0.00003464653],"domain_scores_gemma":[0.99957925,0.000080354745,0.000104765575,0.00008547145,0.000077176686,0.00007297637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003552523,0.0002718009,0.00021030898,0.0009139015,0.00023581451,0.000567244,0.00026599964,0.0002652986,0.0010853828],"category_scores_gemma":[0.0010678973,0.00018009805,0.00030809006,0.00049093436,0.000171547,0.0003806647,0.00027538175,0.00024630985,0.00047670695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007205205,0.00007288507,0.6079715,0.00012206686,0.00015569663,0.0007959775,0.0005524014,0.011439116,0.28351185,0.0047110454,0.0054728542,0.084474064],"study_design_scores_gemma":[0.000036467965,0.00009042674,0.89852357,0.000026952335,0.00004654184,0.00065075594,0.000101242054,0.06258958,0.030418701,0.0013872841,0.006089738,0.00003869952],"about_ca_topic_score_codex":0.0067842617,"about_ca_topic_score_gemma":0.0069614816,"teacher_disagreement_score":0.0067842617,"about_ca_system_score_codex":0.0004905793,"about_ca_system_score_gemma":0.000164494,"threshold_uncertainty_score":0.013489544},"labels":[],"label_agreement":null},{"id":"W3189997181","doi":"10.3847/1538-4357/ac1c78","title":"First Results from HERA Phase I: Upper Limits on the Epoch of Reionization 21 cm Power Spectrum","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":192,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"FP7 International Cooperation; UK Research and Innovation; National Research Foundation; Science and Technology Facilities Council; European Commission; Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Reionization; Physics; HERA; Epoch (astronomy); Astrophysics; Astronomy; Phase (matter); Spectral density; Stars; Galaxy; Particle physics; Redshift","score_opus":0.012752351212895955,"score_gpt":0.2270924019940739,"score_spread":0.21434005078117796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3189997181","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86131084,0.0047760983,0.037916012,0.0010996812,0.00021598178,0.0002716065,0.054209508,0.0016631412,0.038537018],"genre_scores_gemma":[0.92951745,0.0012222033,0.013872543,0.0006828246,0.0002813462,0.0003197645,0.048072744,0.00059338694,0.0054377858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9988809,0.00031316568,0.00004391541,0.00025288446,0.00037882695,0.00013026643],"domain_scores_gemma":[0.9920849,0.0030428052,0.0016383198,0.0017219998,0.0010425386,0.00046944688],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028034067,0.00079821446,0.00046382158,0.0012503369,0.00040860774,0.00096830056,0.00052727835,0.00050497305,0.0037842025],"category_scores_gemma":[0.0048270915,0.0003181084,0.00077470526,0.0008748427,0.00025378447,0.0006507669,0.001259714,0.00048808972,0.0013446234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0029955306,0.00031834858,0.77919257,0.00059807085,0.0010091903,0.00049918704,0.0006795229,0.009952436,0.072562054,0.006910824,0.022571405,0.10271079],"study_design_scores_gemma":[0.00012268285,0.00049233827,0.8974901,0.00008215278,0.00025297888,0.00045354426,0.0001543014,0.0055013136,0.047228277,0.0033664107,0.044773743,0.0000821755],"about_ca_topic_score_codex":0.0017293213,"about_ca_topic_score_gemma":0.0021113267,"teacher_disagreement_score":0.0037842025,"about_ca_system_score_codex":0.0004049987,"about_ca_system_score_gemma":0.00021527923,"threshold_uncertainty_score":0.014826},"labels":[],"label_agreement":null},{"id":"W3190822022","doi":"10.3847/1538-4357/ac5a47","title":"Cosmic Tidal Reconstruction with Halo Fields","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; Canadian Institute for Advanced Research","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Dark matter; Halo; Scale (ratio); Spectral density; Matter power spectrum; Field (mathematics); Anisotropy; Gravitation; Kurtosis; Astrophysics; Classical mechanics; Galaxy; Cosmic microwave background; Optics; Computer science","score_opus":0.005507767197874184,"score_gpt":0.1879045025391768,"score_spread":0.1823967353413026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3190822022","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.46628407,0.00014898746,0.5282823,0.00021592024,0.00004247523,0.000028015545,0.0005612211,0.0017331861,0.002703849],"genre_scores_gemma":[0.8975448,0.000053049556,0.100370996,0.0000349952,0.000012136131,0.00001073642,0.00060109934,0.00015310688,0.0012192116],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999895,0.000026536552,0.000006869322,0.000021794383,0.00003109273,0.000018637349],"domain_scores_gemma":[0.99931335,0.00015377793,0.000091225,0.00020969857,0.0001551751,0.00007672939],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047543898,0.00036772763,0.00023528653,0.0007841076,0.00022315365,0.0006509294,0.0004485477,0.00033059777,0.0015489387],"category_scores_gemma":[0.0025948319,0.0002589266,0.00037218237,0.00058946124,0.0003183174,0.00049732154,0.0005862472,0.0003431459,0.00039325643],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035510014,0.000039170853,0.02088843,0.000041041898,0.00009678483,0.00012579617,0.000108623586,0.8453422,0.017448572,0.012743686,0.0011231783,0.10168747],"study_design_scores_gemma":[0.000010864686,0.000009824679,0.0017598387,0.0000026130513,0.000004667588,0.000022704759,0.000010507083,0.9930529,0.0027508026,0.002021379,0.00034651856,0.000007384947],"about_ca_topic_score_codex":0.0075782165,"about_ca_topic_score_gemma":0.0069121504,"teacher_disagreement_score":0.0075782165,"about_ca_system_score_codex":0.00042271052,"about_ca_system_score_gemma":0.00055575056,"threshold_uncertainty_score":0.015068233},"labels":[],"label_agreement":null},{"id":"W3191238622","doi":"10.3847/1538-4357/ac249c","title":"Supercritical Accretion of Stellar-mass Compact Objects in Active Galactic Nuclei","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Physics; Astrophysics; Accretion (finance); Active galactic nucleus; Outflow; Compact star; Inflow; Eddington luminosity; Neutron star; Stellar mass; White dwarf; Astronomy; Star formation; Stars; Galaxy; Mechanics","score_opus":0.015420578299590215,"score_gpt":0.25281428180231214,"score_spread":0.23739370350272193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3191238622","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.992359,0.0001405804,0.0049316566,0.00003345771,0.0000070843107,0.0000064710225,0.000020923884,0.0000264897,0.0024743793],"genre_scores_gemma":[0.9993788,0.000040000028,0.00030328595,0.0000042691727,0.0000038844273,0.0000020098619,0.000014924612,0.0000023888238,0.00025034993],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99994874,0.000008421129,0.0000029261137,0.00001291993,0.000011784133,0.000015130433],"domain_scores_gemma":[0.9998568,0.00002067591,0.000060052727,0.000018736971,0.000012903745,0.000030795032],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015830286,0.00018468892,0.00022887497,0.00036416698,0.00035334815,0.0005843271,0.00044997016,0.00025331476,0.00045923694],"category_scores_gemma":[0.00035167774,0.0001244097,0.0002968484,0.00012841396,0.00063393754,0.00028961225,0.0005943301,0.00018586619,0.000081763785],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003871756,0.00031100019,0.25648502,0.00019248627,0.0001729316,0.0034124635,0.0007101608,0.46370268,0.16564588,0.086858444,0.0012753056,0.02084643],"study_design_scores_gemma":[0.000030248146,0.00012904427,0.042936843,0.000013347094,0.000034045963,0.0004971935,0.00020933394,0.93248916,0.012803896,0.009580004,0.0012548256,0.00002203445],"about_ca_topic_score_codex":0.0039220243,"about_ca_topic_score_gemma":0.0018995174,"teacher_disagreement_score":0.0039220243,"about_ca_system_score_codex":0.00058501784,"about_ca_system_score_gemma":0.0002329854,"threshold_uncertainty_score":0.0077983737},"labels":[],"label_agreement":null},{"id":"W3192631498","doi":"10.3847/1538-4357/ac1bbb","title":"Bridging the Gap between Protoplanetary and Debris Disks: Separate Evolution of Millimeter and Micrometer-sized Dust","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria; Quest University Canada; Queen's University","funders":"","keywords":"Planetesimal; Debris disk; Physics; Astrophysics; Millimeter; Planet; Debris; Accretion (finance); Protoplanetary disk; Circumstellar dust; Circumstellar disk; Context (archaeology); Astronomy; Cosmic dust; Planetary system; Geology","score_opus":0.017496619714406803,"score_gpt":0.24902549334336505,"score_spread":0.23152887362895824,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3192631498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99825543,0.00074063294,0.00018345915,0.00003511063,0.0000022766521,0.0000026237115,0.0001367324,0.0000043886885,0.0006392615],"genre_scores_gemma":[0.99932516,0.00016058264,0.0002035264,0.000021594777,0.0000051981706,0.0000021935607,0.00012949861,0.0000021812718,0.0001499571],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999256,0.0000072834864,0.0000062410045,0.000026524815,0.000018716133,0.000015691663],"domain_scores_gemma":[0.99964225,0.00008754577,0.00014403222,0.000027966451,0.000041448377,0.000056741563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024437328,0.00010122574,0.0001771352,0.0008781905,0.00029500914,0.0010298103,0.00021125215,0.00020343861,0.0009574125],"category_scores_gemma":[0.0005980557,0.000108260465,0.00011756016,0.00061944214,0.00030058596,0.00044025716,0.00045960853,0.00020063673,0.00014299306],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001767032,0.00003822849,0.94812447,0.00006490469,0.000048774175,0.00020480735,0.00081204594,0.00012961385,0.0313873,0.000424206,0.00014517005,0.018443722],"study_design_scores_gemma":[0.0000011071764,0.00001426976,0.9986218,0.0000067536325,0.000005063575,0.000056010544,0.0002554339,0.00011411361,0.00053551653,0.00008244748,0.00030647797,0.0000010896473],"about_ca_topic_score_codex":0.0018776656,"about_ca_topic_score_gemma":0.0026189736,"teacher_disagreement_score":0.0018776656,"about_ca_system_score_codex":0.00029503138,"about_ca_system_score_gemma":0.00017585838,"threshold_uncertainty_score":0.0037334561},"labels":[],"label_agreement":null},{"id":"W3193666509","doi":"10.3847/1538-4357/ac1ffa","title":"A Sample of Massive Black Holes in Dwarf Galaxies Detected via [Fe x] Coronal Line Emission: Active Galactic Nuclei and/or Tidal Disruption Events","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Experimental Program to Stimulate Competitive Research; High Energy Physics; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; University of Oxford; York University; Max-Planck-Institut für Astrophysik; Nuclear Safety and Security Commission; Leibniz-Gemeinschaft; Montana State University; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Accretion (finance); Population; Astronomy; Dwarf galaxy; Supernova; Line (geometry); Emission spectrum; Supermassive black hole; Spectral line","score_opus":0.020433981994708406,"score_gpt":0.2670415032603882,"score_spread":0.2466075212656798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3193666509","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997002,0.000028464614,0.0000338764,0.0000039890033,4.3699944e-7,0.0000037644863,0.00013720152,0.000002432905,0.00008960996],"genre_scores_gemma":[0.9994153,0.00003200366,0.00007272418,0.000008291105,0.0000033257616,0.0000028872985,0.00037828463,0.0000010243876,0.000086183805],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996989,0.00003428163,0.00003845928,0.00008530887,0.000058852933,0.000084190295],"domain_scores_gemma":[0.99927217,0.00011061586,0.00028141082,0.00007550572,0.00007272278,0.00018766374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003709479,0.00025497118,0.0002479167,0.0014469202,0.00039155787,0.00044739177,0.00020553947,0.00020217472,0.00097604486],"category_scores_gemma":[0.0007137681,0.00014118217,0.00022103566,0.0007432767,0.00035544983,0.00023997543,0.00052579853,0.00011325587,0.00026606533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005490279,0.000027210206,0.99645644,0.00000586599,0.000016685026,0.000102115526,0.000068283,0.000030270332,0.001932852,0.000013647576,0.00004961639,0.0012420125],"study_design_scores_gemma":[0.0000030602223,0.000030412664,0.99918836,0.0000014734,0.000009754133,0.00022619394,0.00009824952,0.00006525515,0.00026701894,0.000006976159,0.00010219949,0.0000010325342],"about_ca_topic_score_codex":0.004342481,"about_ca_topic_score_gemma":0.0060324357,"teacher_disagreement_score":0.004342481,"about_ca_system_score_codex":0.00016054674,"about_ca_system_score_gemma":0.0001543756,"threshold_uncertainty_score":0.008634388},"labels":[],"label_agreement":null},{"id":"W3194160343","doi":"10.3847/1538-4357/ac47fb","title":"The Global Structure of the Milky Way’s Stellar Halo Based on the Orbits of Local Metal-poor Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Japan Society for the Promotion of Science; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Ministry of Education, Culture, Sports, Science and Technology; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Halo; Astrophysics; Milky Way; Stars; Thick disk; Galaxy","score_opus":0.007832078178138165,"score_gpt":0.20587801320695026,"score_spread":0.1980459350288121,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3194160343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99954224,0.00006160531,0.000053754073,0.0000052682935,2.9653137e-7,7.135118e-7,0.00009359146,0.0000041058047,0.00023837455],"genre_scores_gemma":[0.9994967,0.000029448602,0.00006170935,0.000002316643,0.0000014830559,8.0909814e-7,0.00031365562,0.0000030172682,0.000090916976],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993074,0.000007751187,0.000004390649,0.000019525804,0.000014869843,0.000022677888],"domain_scores_gemma":[0.9995414,0.000056860423,0.00013405872,0.00006112987,0.00008711762,0.00011949669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018411977,0.0001467567,0.00020089152,0.0018864959,0.0002273707,0.0006804434,0.00015423316,0.00012667348,0.0008795425],"category_scores_gemma":[0.0006193884,0.00009606035,0.0003425306,0.0011128596,0.0002595717,0.00031359072,0.00087526755,0.000086015825,0.00020271694],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007053078,0.00000660131,0.9901944,0.000008239787,0.00009061428,0.00010069084,0.00021743166,0.0012942604,0.0039955853,0.00012311054,0.00010279956,0.0037957951],"study_design_scores_gemma":[0.0000024412893,0.000014736596,0.9980573,0.000002613537,0.00001867628,0.000052820662,0.00018769085,0.0010956523,0.00031844093,0.000056494973,0.00019019836,0.0000027763017],"about_ca_topic_score_codex":0.0056825113,"about_ca_topic_score_gemma":0.008107484,"teacher_disagreement_score":0.0056825113,"about_ca_system_score_codex":0.0002633076,"about_ca_system_score_gemma":0.00012554672,"threshold_uncertainty_score":0.011298835},"labels":[],"label_agreement":null},{"id":"W3194665130","doi":"10.3847/1538-4357/ac2ffc","title":"HERA Phase I Limits on the Cosmic 21 cm Signal: Constraints on Astrophysics and Cosmology during the Epoch of Reionization","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":161,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"European Research Council; Gordon and Betty Moore Foundation; Science and Technology Facilities Council; National Science Foundation","keywords":"Reionization; Physics; HERA; Cosmology; Astrophysics; Epoch (astronomy); COSMIC cancer database; Astronomy; Stars; Redshift; Galaxy; Particle physics","score_opus":0.013565473845629849,"score_gpt":0.23330758914788896,"score_spread":0.21974211530225912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3194665130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9050729,0.0025984636,0.014097124,0.0025593177,0.00009893125,0.000036580484,0.009246239,0.0005199857,0.06577043],"genre_scores_gemma":[0.99323833,0.00036731717,0.0021302616,0.00022796672,0.00007634356,0.000040483243,0.0024675764,0.00005446889,0.0013971796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966276,0.00010595722,0.00001417312,0.00006832767,0.000093559815,0.00005518466],"domain_scores_gemma":[0.9967025,0.001269331,0.0010456359,0.00036728627,0.00036263512,0.00025273324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020396602,0.00042210674,0.00020746549,0.0012176064,0.00041269325,0.0016784447,0.00036183573,0.00032183272,0.004745934],"category_scores_gemma":[0.0052133356,0.00016084599,0.00027615685,0.00073726417,0.0004084987,0.0009308375,0.0008118833,0.0005019067,0.0009143388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0027228734,0.00017061592,0.6196036,0.0002767928,0.00021240338,0.0004643772,0.0013404709,0.018092377,0.04991413,0.1375633,0.029897545,0.13974148],"study_design_scores_gemma":[0.00014857005,0.00025130407,0.79560244,0.00021163799,0.00009800794,0.00026177432,0.0005497724,0.025894681,0.035845887,0.06456409,0.0764564,0.000115375355],"about_ca_topic_score_codex":0.0030938485,"about_ca_topic_score_gemma":0.0024406025,"teacher_disagreement_score":0.004745934,"about_ca_system_score_codex":0.00058700616,"about_ca_system_score_gemma":0.0002454413,"threshold_uncertainty_score":0.01587671},"labels":[],"label_agreement":null},{"id":"W3194896012","doi":"10.3847/1538-4357/ac0cf1","title":"On the Nature of Organic Dust in Novae","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Japan Society for the Promotion of Science","keywords":"Physics; Astrophysics; Infrared; Nitrogen; Cosmic dust; Condensation; Spectral line; Astrobiology; Galaxy; Circumstellar dust; Infrared spectroscopy; Astrochemistry; Solar System; Astronomy; Interstellar medium","score_opus":0.007337297370826147,"score_gpt":0.22878136019313702,"score_spread":0.22144406282231088,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3194896012","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986089,0.000024256196,0.0002280012,0.000021077805,0.0000036212784,0.000008991533,0.0000618316,0.0000085675565,0.0010347958],"genre_scores_gemma":[0.99966776,0.000013893397,0.00012078733,0.000009280427,0.00000166216,0.0000043599725,0.00006349367,0.0000026119887,0.00011620059],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999267,0.000018614386,0.000002960495,0.00001504789,0.000015156961,0.000021501684],"domain_scores_gemma":[0.999835,0.000065279135,0.000022233293,0.000014613831,0.000015966081,0.00004676078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000152788,0.00023378248,0.00025745155,0.00023566955,0.00042481435,0.00044986187,0.00037636084,0.0005246674,0.0013071127],"category_scores_gemma":[0.0005432076,0.00015198055,0.00038327204,0.00014182416,0.00046063753,0.00025524627,0.00040936877,0.00024532035,0.00011114829],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00074369967,0.0005831187,0.35356852,0.00014717286,0.00030904543,0.001938015,0.00042627976,0.52597713,0.10705143,0.0034640227,0.0006274168,0.005164168],"study_design_scores_gemma":[0.00027787217,0.00075049064,0.34885597,0.000020835323,0.00005725364,0.00031016654,0.0007462068,0.63256633,0.0125228735,0.0021393348,0.0016970757,0.00005557687],"about_ca_topic_score_codex":0.0045512416,"about_ca_topic_score_gemma":0.002210887,"teacher_disagreement_score":0.0045512416,"about_ca_system_score_codex":0.00046078948,"about_ca_system_score_gemma":0.00018639133,"threshold_uncertainty_score":0.009049475},"labels":[],"label_agreement":null},{"id":"W3195074751","doi":"10.3847/1538-4357/ac1e8d","title":"Physical Drivers of Emission-line Diversity of SDSS Seyfert 2s and LINERs after Removal of Contributions from Star Formation","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Astrophysics; Ionization; Metallicity; Physics; Line (geometry); Star (game theory); Emission spectrum; Star formation; Stars; Astronomy; Spectral line; Geometry","score_opus":0.010693435132489496,"score_gpt":0.2467091513519534,"score_spread":0.2360157162194639,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3195074751","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997391,0.0000151617805,0.000054565884,0.0000072612197,7.307824e-7,9.0072433e-7,0.00009222832,0.0000062140793,0.00008373885],"genre_scores_gemma":[0.99937326,0.000006763989,0.00006483347,0.0000044800536,0.0000021853746,0.000002173865,0.00042387182,0.0000063680595,0.00011611707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969304,0.00003279059,0.000018218265,0.00012624293,0.000054134467,0.00007566124],"domain_scores_gemma":[0.99803835,0.00045788265,0.0007364959,0.00024502396,0.00022799135,0.0002943744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00073104934,0.0002684104,0.00049075653,0.0015076869,0.00053833134,0.0009941871,0.0003475613,0.0003957304,0.0020075592],"category_scores_gemma":[0.0025048875,0.00017596658,0.00040358907,0.0009858533,0.00045121342,0.00046191487,0.00057592656,0.00032914328,0.00046072557],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011840598,0.00002511324,0.9894796,0.000005991131,0.000068091525,0.00010856429,0.00022500321,0.00046220922,0.0065748743,0.00013675718,0.00016199728,0.002633291],"study_design_scores_gemma":[0.000003522121,0.000010172339,0.9981487,0.0000021891133,0.000009838339,0.00003726992,0.00010766827,0.0012222418,0.0002819958,0.00004809573,0.00012643002,0.0000019165007],"about_ca_topic_score_codex":0.0055916826,"about_ca_topic_score_gemma":0.0065236543,"teacher_disagreement_score":0.0055916826,"about_ca_system_score_codex":0.00054020254,"about_ca_system_score_gemma":0.0001719484,"threshold_uncertainty_score":0.011118293},"labels":[],"label_agreement":null},{"id":"W3195676520","doi":"10.3847/1538-4357/ac09ed","title":"Characterization of HD 206893 B from Near- to Thermal-infrared","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"European Research Council; European Commission; Space Telescope Science Institute; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation","keywords":"Brown dwarf; Physics; Astrophysics; Proper motion; Debris disk; Orbital motion; Astronomy; Planet; Planetary system; Stars; Angular momentum","score_opus":0.009121263233193342,"score_gpt":0.21172657555363805,"score_spread":0.2026053123204447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3195676520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897655,0.000277405,0.0005419566,0.00009573649,0.00003069207,0.000022229837,0.0033232297,0.00012629398,0.005817043],"genre_scores_gemma":[0.9930347,0.00007053983,0.0012736736,0.00010770851,0.000022777536,0.000014502592,0.0046457937,0.00003238604,0.00079805084],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999051,0.00000590942,0.000005785689,0.000028438373,0.000033911212,0.000020856896],"domain_scores_gemma":[0.9997125,0.000014593644,0.00007399492,0.000025852523,0.00005095825,0.00012197476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011445085,0.0002110486,0.00022309048,0.0011606462,0.00045107558,0.00030989706,0.00019333443,0.0003011987,0.0017492806],"category_scores_gemma":[0.00016946891,0.00015267498,0.00019353234,0.0007981616,0.00015939555,0.00011609135,0.00022685598,0.00024798952,0.001404189],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008585533,0.00033084652,0.63454,0.0001351715,0.00008409824,0.0012251361,0.00033616586,0.0006239512,0.33078474,0.00065275066,0.00830489,0.022123734],"study_design_scores_gemma":[0.000017927716,0.000068590656,0.9883454,0.000008121509,0.00001368096,0.000497661,0.00008090483,0.00082003337,0.005861252,0.0000734169,0.004204625,0.000008394839],"about_ca_topic_score_codex":0.0055777957,"about_ca_topic_score_gemma":0.010099145,"teacher_disagreement_score":0.0055777957,"about_ca_system_score_codex":0.0002698422,"about_ca_system_score_gemma":0.0001491964,"threshold_uncertainty_score":0.011090696},"labels":[],"label_agreement":null},{"id":"W3195701015","doi":"10.3847/1538-4357/ac1f20","title":"Resolving the Fastest Ejecta from Binary Neutron Star Mergers: Implications for Electromagnetic Counterparts","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Aeronautics and Space Administration","keywords":"Ejecta; Kilonova; Physics; Neutron star; Astrophysics; RADIUS; Gravitational wave; Binary number; Computational physics; Supernova","score_opus":0.016093068484991636,"score_gpt":0.25150909582326786,"score_spread":0.2354160273382762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3195701015","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99426526,0.00012075702,0.0038571921,0.00012338864,0.00001106467,0.0000067464007,0.000083186926,0.000059150883,0.0014733147],"genre_scores_gemma":[0.9969861,0.000052247564,0.0027087075,0.000019239988,0.0000043864197,0.0000044294998,0.000063209736,0.00001955293,0.00014214366],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999013,0.000031580672,0.00000566843,0.00001721312,0.000026949932,0.000017188791],"domain_scores_gemma":[0.99883527,0.00072324014,0.00016281969,0.00009920076,0.00008410634,0.00009544595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004939512,0.00031133095,0.00033463092,0.00027302888,0.00040155355,0.00085768977,0.0004725417,0.0003489662,0.0011571815],"category_scores_gemma":[0.0037987789,0.00022319621,0.00026074817,0.00029615697,0.00045771105,0.0005247947,0.0005311212,0.00033508264,0.00011285235],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006430353,0.00016543611,0.06017267,0.00009678558,0.00009102366,0.0003873528,0.00018847774,0.9011109,0.02299479,0.0051089777,0.00039772713,0.008642829],"study_design_scores_gemma":[0.00007664795,0.000111078945,0.014195358,0.000009550236,0.000018430557,0.000075934935,0.000097208715,0.9759469,0.0070822663,0.0019664776,0.00040578365,0.000014409966],"about_ca_topic_score_codex":0.0038464225,"about_ca_topic_score_gemma":0.0026382895,"teacher_disagreement_score":0.0038464225,"about_ca_system_score_codex":0.00040400945,"about_ca_system_score_gemma":0.0002790949,"threshold_uncertainty_score":0.0076481104},"labels":[],"label_agreement":null},{"id":"W3195804136","doi":"10.3847/1538-4357/ac214d","title":"Optical and Near-infrared Pulsation Properties of RR Lyrae and Population II Cepheid Variables in the Messier 15 Globular Cluster","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"RR Lyrae variable; Cepheid variable; Globular cluster; Astrophysics; Physics; Variable star; Metallicity; Distance modulus; Population; Astronomy; Luminosity; Light curve; Stars; Galaxy; Medicine","score_opus":0.013396669839960941,"score_gpt":0.22072815859967218,"score_spread":0.20733148875971125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3195804136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996068,0.000027730686,0.000013931516,0.000004824536,3.7859203e-7,9.948276e-7,0.00014759933,0.000003246032,0.00019453165],"genre_scores_gemma":[0.9991385,0.000025394978,0.00007612404,0.0000068480726,0.0000027644057,0.0000021188116,0.0005091789,0.0000025844024,0.00023657734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994695,0.0000032051157,0.000003734175,0.000023006518,0.000009589126,0.000013568953],"domain_scores_gemma":[0.9998381,0.000017863646,0.000075637516,0.0000102583845,0.00001164912,0.00004637606],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000090692236,0.00018917207,0.000135629,0.0007285376,0.00015918382,0.0002548149,0.00014467741,0.00009734005,0.001070823],"category_scores_gemma":[0.00025966082,0.00007481012,0.00009666951,0.00032017005,0.00013988075,0.00013907425,0.00022643738,0.000090056834,0.00022605062],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017702108,0.000021170037,0.98287404,0.000008169377,0.000029815443,0.000121485326,0.00028936245,0.00023626581,0.011045859,0.000103098646,0.00036716595,0.0047264886],"study_design_scores_gemma":[0.000002697952,0.000014610786,0.999255,0.0000010824889,0.000005165369,0.00003002723,0.000034813995,0.00015482519,0.00032683258,0.00000883406,0.00016453791,0.0000015728596],"about_ca_topic_score_codex":0.024003986,"about_ca_topic_score_gemma":0.038639996,"teacher_disagreement_score":0.024003986,"about_ca_system_score_codex":0.00038992063,"about_ca_system_score_gemma":0.000061539,"threshold_uncertainty_score":0.04772854},"labels":[],"label_agreement":null},{"id":"W3196095052","doi":"10.3847/1538-4357/ac20da","title":"Circumstellar Medium Constraints on the Environment of Two Nearby Type Ia Supernovae: SN 2017cbv and SN 2020nlb","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"","keywords":"Physics; Supernova; Astrophysics; RADIUS; Type (biology); Luminosity; White dwarf; Degenerate energy levels; Lambda; Stars; Galaxy","score_opus":0.016794632838403725,"score_gpt":0.2437969138348679,"score_spread":0.2270022809964642,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3196095052","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972187,0.00025359495,0.00037184224,0.000025692321,0.000010593931,0.0000035683747,0.00021424517,0.000025592084,0.001876168],"genre_scores_gemma":[0.9986952,0.000058963305,0.00029274414,0.000020302978,0.0000068718387,0.0000046101786,0.0007239706,0.000013213706,0.00018407426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980825,0.000019345707,0.000011403741,0.0000427612,0.00005986661,0.000058415415],"domain_scores_gemma":[0.99895716,0.00015594122,0.00026743673,0.000087932276,0.000136822,0.00039464814],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052683346,0.00039072378,0.0005673968,0.0010237708,0.0006297796,0.001694751,0.0005062273,0.00039332148,0.0014067836],"category_scores_gemma":[0.0011753988,0.00035139988,0.00031507414,0.00041008726,0.00051447924,0.00036466672,0.0010353837,0.00030039117,0.00054187136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012503088,0.00017731907,0.78314906,0.00010147059,0.00016878742,0.0020029664,0.00036621292,0.003585493,0.19840534,0.001979938,0.0009620085,0.007851205],"study_design_scores_gemma":[0.0000954847,0.00021996348,0.95561236,0.00004599582,0.000106275314,0.0012784188,0.0008184377,0.013023111,0.021960402,0.0012286521,0.0055519165,0.00005908989],"about_ca_topic_score_codex":0.007863668,"about_ca_topic_score_gemma":0.012019745,"teacher_disagreement_score":0.007863668,"about_ca_system_score_codex":0.0006288356,"about_ca_system_score_gemma":0.0004517346,"threshold_uncertainty_score":0.015635788},"labels":[],"label_agreement":null},{"id":"W3196406579","doi":"10.3847/1538-4357/ac21cc","title":"Detection of Substructures in Young Transition Disk WL 17","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Substructure; Ophiuchus; Physics; Polarization (electrochemistry); Astrophysics; Scattering; Optics; Star formation; Stars","score_opus":0.007425473688960846,"score_gpt":0.22901064553663125,"score_spread":0.2215851718476704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3196406579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999363,0.0000377036,0.00019998476,0.000008462515,0.000001405313,0.0000022042655,0.00012346888,0.000019218367,0.00024461016],"genre_scores_gemma":[0.99950325,0.0000145430095,0.00022555748,0.0000071070544,0.0000019626566,0.0000025937575,0.00019228773,0.0000041100634,0.000048568738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999316,0.0000049289033,0.000004127154,0.00002265277,0.000015423027,0.000021321526],"domain_scores_gemma":[0.99964404,0.00004037952,0.00013137101,0.000027550046,0.000041850573,0.00011486775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110103014,0.00022676797,0.00017694716,0.00073506584,0.00029624873,0.00037693404,0.00026768385,0.00023420101,0.0008363564],"category_scores_gemma":[0.00027335004,0.00016212107,0.00015583562,0.0003556732,0.00020243939,0.00016749823,0.0003453974,0.00020297804,0.00024637752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010653465,0.00003225859,0.9204135,0.000026643089,0.0000377551,0.0002729337,0.00024170121,0.0001721943,0.07303121,0.0001011916,0.0001811039,0.0053829583],"study_design_scores_gemma":[0.000007127042,0.00008090123,0.9936779,0.0000066788784,0.000019798377,0.00026884567,0.00018980459,0.00053018663,0.0046232035,0.000051329484,0.0005391685,0.000005126938],"about_ca_topic_score_codex":0.0019020566,"about_ca_topic_score_gemma":0.0036592449,"teacher_disagreement_score":0.0019020566,"about_ca_system_score_codex":0.00024053047,"about_ca_system_score_gemma":0.000071177106,"threshold_uncertainty_score":0.0037819743},"labels":[],"label_agreement":null},{"id":"W3196911878","doi":"10.3847/1538-4357/ac2360","title":"Discovery of ASKAP J173608.2–321635 as a Highly Polarized Transient Point Source with the Australian SKA Pathfinder","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council; Science and Technology Facilities Council","keywords":"Pulsar; Pathfinder; Telescope; Point source; Source counts; Galactic Center; Polarization (electrochemistry); Observatory; Galaxy","score_opus":0.009642079888382064,"score_gpt":0.2168089693200391,"score_spread":0.20716688943165704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3196911878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982571,0.000074761134,0.0002816595,0.00007318897,0.000014628847,0.000011314036,0.00017629619,0.000019275984,0.0010918335],"genre_scores_gemma":[0.9979564,0.000048400332,0.00067223073,0.000043543045,0.000019906809,0.000012189974,0.00044849585,0.000007318935,0.0007914818],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974006,0.000018156747,0.000015333613,0.00005601474,0.00011580077,0.00005450077],"domain_scores_gemma":[0.99944323,0.000037890684,0.00014196702,0.00007306338,0.00008644931,0.00021724982],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000338567,0.00028859294,0.00032950874,0.0011273108,0.0009089837,0.0007547138,0.00046480994,0.00064362393,0.0011777023],"category_scores_gemma":[0.00047846098,0.00028059594,0.0003782683,0.000833033,0.00059764605,0.00028133314,0.0012427162,0.00061334413,0.0005645821],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005381409,0.00020878678,0.7341391,0.00013589888,0.00014892516,0.018891465,0.0034044457,0.00056146766,0.20990013,0.001075958,0.0025831528,0.028412582],"study_design_scores_gemma":[0.000020959225,0.00022266289,0.9815916,0.000023538116,0.000043821095,0.0049992697,0.0005114489,0.00086357107,0.0049807336,0.00032720118,0.0063871727,0.00002806637],"about_ca_topic_score_codex":0.0042446856,"about_ca_topic_score_gemma":0.0044960952,"teacher_disagreement_score":0.0042446856,"about_ca_system_score_codex":0.00036100985,"about_ca_system_score_gemma":0.00029616937,"threshold_uncertainty_score":0.008439958},"labels":[],"label_agreement":null},{"id":"W3197199081","doi":"10.3847/1538-4357/ac3423","title":"Determination of Sodium Abundance Ratio from Low-resolution Stellar Spectra and Its Applications","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Leibniz-Gemeinschaft; University of Notre Dame; Ohio State University; National Research Foundation; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; National Science Foundation; Lawrence Berkeley National Laboratory; Ministry of Science and ICT, South Korea; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Stars; Physics; Astrophysics; Metallicity; Spectral line; Galactic halo; Halo; Extinction (optical mineralogy); Interstellar medium; Astronomy; Galaxy","score_opus":0.008738836377604278,"score_gpt":0.21888813860670714,"score_spread":0.21014930222910286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3197199081","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5498919,0.002201753,0.43378657,0.000120170305,0.00006727309,0.00015960111,0.0013546159,0.004528937,0.007889131],"genre_scores_gemma":[0.6783786,0.0004564094,0.31831232,0.00004179496,0.000024631832,0.00008286309,0.00075263437,0.0001601358,0.0017905998],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9995983,0.000054829066,0.000038180096,0.00014519246,0.00014494923,0.000018691977],"domain_scores_gemma":[0.9993741,0.00010020011,0.00013126503,0.00008773406,0.00025896312,0.000047738948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006636278,0.00037409188,0.0003665202,0.0018438605,0.00031306053,0.0005298001,0.00068041135,0.00039395696,0.0013725942],"category_scores_gemma":[0.0015071735,0.00027153725,0.0002538699,0.0008169627,0.00017337974,0.0005293677,0.00044944353,0.00025348243,0.001246901],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002796876,0.00011218663,0.16687891,0.00033936964,0.00012579306,0.0001856268,0.00015969071,0.0034197345,0.6258233,0.0008079973,0.00047826188,0.20138943],"study_design_scores_gemma":[0.00006309049,0.00032952978,0.21802285,0.000080279395,0.00015434847,0.0012941095,0.00027195102,0.14936468,0.6154103,0.0024777236,0.012376232,0.00015493752],"about_ca_topic_score_codex":0.001025294,"about_ca_topic_score_gemma":0.0018503969,"teacher_disagreement_score":0.0018438605,"about_ca_system_score_codex":0.00017983053,"about_ca_system_score_gemma":0.00016154534,"threshold_uncertainty_score":0.0045918226},"labels":[],"label_agreement":null},{"id":"W3197470584","doi":"10.3847/1538-4357/ac390b","title":"Galactic Mass Estimates Using Dwarf Galaxies as Kinematic Tracers","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; National Science Foundation","keywords":"Milky Way; Galaxy; Astrophysics; Physics; Dwarf galaxy; Globular cluster; Gravitational potential; Large Magellanic Cloud; Bayesian probability; Estimator; Sensitivity (control systems); Local Group; Statistics; Mathematics","score_opus":0.016209951672613496,"score_gpt":0.248359178223726,"score_spread":0.2321492265511125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3197470584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84920263,0.0011217541,0.13815475,0.00018984724,0.000017876533,0.000036789705,0.0019630536,0.00095263706,0.008360667],"genre_scores_gemma":[0.9900594,0.00010809733,0.0085085975,0.000015241253,0.000009294304,0.000010255627,0.000996857,0.000041554347,0.00025065785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994055,0.00018417268,0.00003020544,0.00019259853,0.0001486496,0.000038754788],"domain_scores_gemma":[0.9955511,0.0023028837,0.00078126974,0.00071475975,0.00054334896,0.00010672963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024323158,0.0004529022,0.00035910393,0.0027264678,0.00018477716,0.0013299336,0.00079574774,0.00044272988,0.0009430558],"category_scores_gemma":[0.015688915,0.00026873767,0.0004889516,0.00089228357,0.0004911227,0.0010461615,0.0010046284,0.00038334972,0.0004341562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002680562,0.000024753901,0.5639481,0.00008916144,0.0005762927,0.00014401849,0.00041163596,0.33872136,0.0045841066,0.026562862,0.0016344597,0.06303529],"study_design_scores_gemma":[0.000075632226,0.00008533015,0.26486853,0.00014096056,0.0001715975,0.00029892792,0.00027051085,0.67386466,0.01112738,0.04013383,0.008822951,0.00013973466],"about_ca_topic_score_codex":0.009423618,"about_ca_topic_score_gemma":0.0041008014,"teacher_disagreement_score":0.009423618,"about_ca_system_score_codex":0.00081459177,"about_ca_system_score_gemma":0.00021654407,"threshold_uncertainty_score":0.018737495},"labels":[],"label_agreement":null},{"id":"W3197578311","doi":"10.3847/1538-4357/ac2576","title":"Discovery of Eight “Main-sequence Radio Pulse Emitters” Using the GMRT: Clues to the Onset of Coherent Radio Emission in Hot Magnetic Stars","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomical Observations and Instrumentation","field":"Engineering","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University; Royal Military College of Canada","funders":"","keywords":"Astrophysics; Physics; Stars; Giant Metrewave Radio Telescope; Magnetic field; Maser; Astronomy; Galaxy; Radio galaxy","score_opus":0.02226617929758048,"score_gpt":0.24887955512536325,"score_spread":0.22661337582778276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3197578311","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99748355,0.00025301456,0.0013676703,0.00003175346,0.000006054472,0.0000074422005,0.00011441461,0.000031352203,0.00070472935],"genre_scores_gemma":[0.9979868,0.00007589263,0.001549791,0.000029059078,0.000017677508,0.0000052717915,0.00019436852,0.000010240885,0.0001307779],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998801,0.000013854084,0.000009575124,0.000046541365,0.000028202045,0.000021748816],"domain_scores_gemma":[0.99931955,0.00013803001,0.00024750922,0.00007948613,0.00008537863,0.00012997299],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037470896,0.00016397721,0.00021140931,0.0008517182,0.00026530997,0.0004892701,0.00024524552,0.00039802538,0.00073753856],"category_scores_gemma":[0.0007451881,0.00015498769,0.00021294378,0.00043475584,0.00024642944,0.00025638725,0.00045596174,0.0003018611,0.0004290692],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003081447,0.00007451404,0.782014,0.000105870764,0.000102891856,0.0011643231,0.00037019298,0.00026246908,0.19371322,0.00038878838,0.00030349148,0.021192033],"study_design_scores_gemma":[0.00001309177,0.00019713321,0.98067296,0.000015381422,0.0000588935,0.0017728163,0.00015710312,0.0013456945,0.014110058,0.00025890488,0.0013851792,0.000012705301],"about_ca_topic_score_codex":0.00017460877,"about_ca_topic_score_gemma":0.00031714304,"teacher_disagreement_score":0.0008517182,"about_ca_system_score_codex":0.00010137209,"about_ca_system_score_gemma":0.000058603557,"threshold_uncertainty_score":0.0024673343},"labels":[],"label_agreement":null},{"id":"W3198131901","doi":"10.3847/1538-4357/ac2237","title":"Discovery of a 310 Day Period from the Enshrouded Massive System NaSt1 (WR 122)","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; Deutsches Elektronen-Synchrotron; Center for Cosmology and Astroparticle Physics, Ohio State University; Stockholms Universitet; Chinese Academy of Sciences; University of New South Wales; Science and Technology Facilities Council; Weizmann Institute of Science; Chinese Academy of Sciences South America Center for Astronomy; Australian Government; Villum Fonden; Space Telescope Science Institute; National Science Foundation; University of Washington; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; California Institute of Technology; Ohio State University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation","keywords":"Light curve; Physics; Astrophysics; Astronomy; Orbital period; Amplitude; Supernova; Photometry (optics); Wavelength; Asteroid; Infrared; Stars; Optics","score_opus":0.010916168531335821,"score_gpt":0.22222844979419634,"score_spread":0.21131228126286053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3198131901","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980106,0.00007491395,0.00020653062,0.000047775902,0.000016083233,0.000007020785,0.00031172615,0.000027314467,0.0012980516],"genre_scores_gemma":[0.998743,0.000027766,0.00023956262,0.000023163968,0.000021195743,0.0000049240025,0.0006571589,0.000005274911,0.00027802182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993277,0.000004239263,0.000004536924,0.000025084502,0.000019053461,0.000014333121],"domain_scores_gemma":[0.9997191,0.000013895542,0.00010524281,0.000023610146,0.000035959583,0.00010221731],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001932808,0.00018715176,0.00018811696,0.0008650433,0.0008032646,0.0005044143,0.00022439731,0.00026494925,0.0010280713],"category_scores_gemma":[0.00034200787,0.00013912345,0.00014914763,0.00050691486,0.00030417394,0.0002833631,0.0005976207,0.00044745917,0.00033835886],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069855637,0.00019539196,0.8331487,0.000086692424,0.000076774326,0.0051313206,0.0011922432,0.00043793427,0.13020672,0.00093916757,0.0022433877,0.025642991],"study_design_scores_gemma":[0.000006278641,0.00009736257,0.99496067,0.000006875933,0.000008949607,0.0009214579,0.000098688906,0.00035577186,0.0014656661,0.00008553587,0.0019874545,0.0000053394133],"about_ca_topic_score_codex":0.0018926383,"about_ca_topic_score_gemma":0.004224938,"teacher_disagreement_score":0.0018926383,"about_ca_system_score_codex":0.000489323,"about_ca_system_score_gemma":0.00012852176,"threshold_uncertainty_score":0.0037631989},"labels":[],"label_agreement":null},{"id":"W3198614206","doi":"10.3847/1538-4357/ac4494","title":"Bayesian Inference of Globular Cluster Properties Using Distribution Functions","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Globular cluster; Cluster (spacecraft); Bayesian inference; Bayesian probability; Statistical inference; Bayesian hierarchical modeling; Stars; Inference; Physics; Statistics; Computer science; Mathematics; Algorithm; Astrophysics; Artificial intelligence","score_opus":0.018552099400159283,"score_gpt":0.228272857033145,"score_spread":0.20972075763298573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3198614206","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.31257716,0.0002041202,0.68448246,0.00037855303,0.00001753792,0.00008062304,0.00046835467,0.00053969095,0.0012514233],"genre_scores_gemma":[0.94242406,0.000120691075,0.05569898,0.000090817346,0.00003528001,0.00005143399,0.0009196546,0.00010367463,0.0005554411],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9973808,0.0015622003,0.000075272736,0.0005447222,0.00026480443,0.00017215991],"domain_scores_gemma":[0.9689085,0.025352405,0.0017476622,0.0018660432,0.0015715233,0.0005538188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.011413399,0.0007149898,0.0011753668,0.0030682846,0.0010436906,0.0023479918,0.0024251842,0.0013030266,0.0015236528],"category_scores_gemma":[0.05955068,0.0008865462,0.0010622639,0.0014772726,0.0023009672,0.0025332067,0.0011854859,0.0016442084,0.0003487332],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001251132,0.000054583423,0.030444613,0.000033780096,0.00015075912,0.0000775761,0.00014264061,0.92262924,0.00094056653,0.03103244,0.0007325168,0.013636211],"study_design_scores_gemma":[0.000012454431,0.000008358018,0.0034291865,0.00001210491,0.000010418627,0.000013789742,0.000017686987,0.9771482,0.00034038228,0.018854804,0.00013454416,0.000018024226],"about_ca_topic_score_codex":0.033425916,"about_ca_topic_score_gemma":0.021570463,"teacher_disagreement_score":0.033425916,"about_ca_system_score_codex":0.0029804816,"about_ca_system_score_gemma":0.0014140873,"threshold_uncertainty_score":0.066462755},"labels":[],"label_agreement":null},{"id":"W3198704240","doi":"10.3847/1538-4357/ac3978","title":"Probing Extremal Gravitational-wave Events with Coarse-grained Likelihoods","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Ministry of Colleges and Universities; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; Space Telescope Science Institute; Government of Canada; National Science Foundation","keywords":"Physics; LIGO; Astrophysics; Binary black hole; Gravitational wave; Population; Black hole (networking); Outlier; Neutron star; Binary number; Astronomy; Statistics","score_opus":0.016722686423292166,"score_gpt":0.2881300219368758,"score_spread":0.27140733551358365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3198704240","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86822146,0.00017772676,0.12718134,0.00025015135,0.00002200867,0.000071554416,0.0014047476,0.0011500851,0.0015209013],"genre_scores_gemma":[0.98501194,0.000014693893,0.013516365,0.000031303232,0.000024352492,0.00002035274,0.0011312914,0.000058505346,0.00019131169],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99788254,0.0007414921,0.00018842192,0.0005827008,0.00033016235,0.00027474118],"domain_scores_gemma":[0.9623111,0.026081327,0.0040220604,0.005514902,0.0009849953,0.0010857171],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.006837911,0.00039468752,0.0008588331,0.004698972,0.0010503503,0.00234412,0.0012956816,0.000923503,0.0034974127],"category_scores_gemma":[0.034199387,0.00037724554,0.0008506528,0.0020287982,0.0011942004,0.002479671,0.0031264175,0.0013921626,0.0004542551],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062978343,0.0002948438,0.7362835,0.00013533041,0.0003973341,0.0003515614,0.0008198273,0.16385987,0.006615665,0.0161194,0.0023108814,0.07218207],"study_design_scores_gemma":[0.000052098072,0.000104129336,0.22162865,0.000032065578,0.00008010307,0.00018566867,0.00031171518,0.7484294,0.0029925925,0.024308389,0.0017984724,0.00007668561],"about_ca_topic_score_codex":0.006392747,"about_ca_topic_score_gemma":0.0072898604,"teacher_disagreement_score":0.006837911,"about_ca_system_score_codex":0.0008785759,"about_ca_system_score_gemma":0.0005010749,"threshold_uncertainty_score":0.036162734},"labels":[],"label_agreement":null},{"id":"W3198924935","doi":"10.3847/1538-4357/ac9f14","title":"Inpainting Hydrodynamical Maps with Deep Learning","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Division of Astronomical Sciences","keywords":"Physics; Missing data; Inpainting; Offset (computer science); Pixel; Convolutional neural network; Astrophysics; Spectral density; Deep learning; Projection (relational algebra); Artificial intelligence; Galaxy; Pattern recognition (psychology); Statistical physics; Algorithm; Image (mathematics); Statistics; Computer science; Optics; Mathematics","score_opus":0.0037467594165374167,"score_gpt":0.18374828820231842,"score_spread":0.18000152878578102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3198924935","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75633913,0.00063217,0.22648469,0.0008778352,0.00040231177,0.00008179425,0.0022716713,0.009963282,0.002947158],"genre_scores_gemma":[0.9466776,0.000085267005,0.05045399,0.00015106396,0.00004953888,0.000028557712,0.0015751085,0.00027721154,0.0007016436],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998816,0.000017457203,0.000005045638,0.00003119895,0.000038901588,0.000025870808],"domain_scores_gemma":[0.99946874,0.00024043643,0.000065765715,0.00009625977,0.00008259408,0.000046200832],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004730501,0.0008475347,0.0005606381,0.00060694077,0.00021460008,0.0005176698,0.0011116836,0.0007906458,0.0017725722],"category_scores_gemma":[0.001984551,0.00041227508,0.00076668063,0.00039884317,0.0005859427,0.00042854983,0.0005898044,0.00087786803,0.00024850218],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015489687,0.000046156758,0.002052153,0.00006667212,0.00006591591,0.00015299492,0.00004631037,0.9764997,0.0040703216,0.0005286761,0.0017693744,0.014546775],"study_design_scores_gemma":[0.000020479047,0.000021790209,0.0005553846,0.000005441342,0.000007460378,0.000020133592,0.000008195169,0.99626476,0.0022228777,0.000595641,0.00027269585,0.0000051582037],"about_ca_topic_score_codex":0.007131132,"about_ca_topic_score_gemma":0.0062040635,"teacher_disagreement_score":0.007131132,"about_ca_system_score_codex":0.00052869885,"about_ca_system_score_gemma":0.00049328915,"threshold_uncertainty_score":0.01417923},"labels":[],"label_agreement":null},{"id":"W3199004861","doi":"10.3847/1538-4357/ac27a7","title":"What is Important? Morphological Asymmetries are Useful Predictors of Star Formation Rates of Star-forming Galaxies in SDSS Stripe 82","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Natural Science Foundation of China; York University; Office of Science; Johns Hopkins University; National Key Research and Development Program of China; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Bulge; Star formation; Galaxy; Star (game theory); Asymmetry; Redshift; Sky; Stellar mass; Astronomy","score_opus":0.013233866980537958,"score_gpt":0.22931712308262664,"score_spread":0.21608325610208867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199004861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998582,0.000107105836,0.0005320366,0.00016740554,0.0000029081332,0.0000015614287,0.00018596546,0.000022725404,0.00039830751],"genre_scores_gemma":[0.9996841,0.000016557062,0.0001105796,0.000010788506,0.000011320553,4.1408978e-7,0.00012492653,0.000002909228,0.00003848722],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996088,0.00014865828,0.000026716174,0.00008705547,0.000056815035,0.00007201607],"domain_scores_gemma":[0.99390864,0.0029144099,0.0017551208,0.00031433871,0.00033135683,0.0007761516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012927228,0.00031032073,0.00043245687,0.0009814696,0.00032001198,0.0012444017,0.00029835216,0.00053707336,0.0012365215],"category_scores_gemma":[0.007349576,0.00019959625,0.00030056134,0.00087347464,0.00056073535,0.0009367406,0.0006520678,0.0005704932,0.00028641056],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007709595,0.000012433035,0.99384415,0.000008867442,0.000044154414,0.000022810784,0.000032032684,0.0011186814,0.00076659495,0.00011488829,0.00016374125,0.0037946417],"study_design_scores_gemma":[0.000006829386,0.00003336862,0.9839474,0.0000066661787,0.000028603652,0.000046287456,0.0001252906,0.014646013,0.0004877339,0.0005184709,0.00014550814,0.000007798616],"about_ca_topic_score_codex":0.00256245,"about_ca_topic_score_gemma":0.0036696207,"teacher_disagreement_score":0.00256245,"about_ca_system_score_codex":0.0002458275,"about_ca_system_score_gemma":0.00022000792,"threshold_uncertainty_score":0.0068366528},"labels":[],"label_agreement":null},{"id":"W3199721451","doi":"10.3847/1538-4357/ac2363","title":"Perpendicular Diffusion of Energetic Particles: A Complete Analytical Theory","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Perpendicular; Physics; Turbulence; Statistical physics; Diffusion; Limit (mathematics); Random walk; Test particle; Magnetic field; Diffusion process; Classical mechanics; Mechanics; Mathematics; Mathematical analysis; Geometry; Quantum mechanics; Computer science; Statistics","score_opus":0.008638403880508723,"score_gpt":0.22581777543742673,"score_spread":0.21717937155691802,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199721451","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.092004776,0.002109007,0.8483456,0.0010698906,0.0004920438,0.000101154976,0.00019673597,0.00027731707,0.055403523],"genre_scores_gemma":[0.902582,0.0027048164,0.053465042,0.0004412084,0.00043330743,0.00016660019,0.00018324921,0.00020037394,0.039823417],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997701,0.000043862132,0.000012427994,0.000040823183,0.00010419724,0.000028624114],"domain_scores_gemma":[0.99969864,0.000080887585,0.000049516606,0.000036283272,0.0001042547,0.000030369809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043818008,0.0006835053,0.0006704329,0.0012288223,0.000532847,0.0010392868,0.0009957659,0.0007769291,0.0025817181],"category_scores_gemma":[0.0011262059,0.00027079965,0.00065008376,0.00044880624,0.0014755003,0.0020323233,0.0010918997,0.00093052094,0.0005292832],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029940742,0.0000594633,0.00048023064,0.00012207094,0.00001867874,0.00017749923,0.00010394436,0.123911485,0.0080747595,0.85779023,0.0017957055,0.0074358336],"study_design_scores_gemma":[0.000008794569,0.000023617984,0.00018509114,0.000014150201,0.000005945388,0.000100017285,0.000021874417,0.87497103,0.0007548657,0.12154193,0.002356699,0.000016016613],"about_ca_topic_score_codex":0.0022096983,"about_ca_topic_score_gemma":0.0006848726,"teacher_disagreement_score":0.0025817181,"about_ca_system_score_codex":0.0008356913,"about_ca_system_score_gemma":0.0006891727,"threshold_uncertainty_score":0.008636713},"labels":[],"label_agreement":null},{"id":"W3199735555","doi":"10.3847/1538-4357/ac35d6","title":"Functional Data Analysis for Extracting the Intrinsic Dimensionality of Spectra: Application to Chemical Homogeneity in the Open Cluster M67","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Office of Science; University of Utah; Alfred P. Sloan Foundation; U.S. Department of Energy","keywords":"Physics; Principal component analysis; Astrophysics; Cluster (spacecraft); Spectral line; Stars; Open cluster; Curse of dimensionality; Artificial intelligence; Computer science; Astronomy","score_opus":0.05057186045149653,"score_gpt":0.31407172473763323,"score_spread":0.2634998642861367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199735555","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8714059,0.0001777854,0.12610325,0.0003045965,0.000008987289,0.00003414082,0.0006013072,0.00058582163,0.00077814417],"genre_scores_gemma":[0.9657981,0.00003755844,0.033336606,0.000021188991,0.000011459922,0.000018679453,0.00063822255,0.0000498701,0.000088266],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99946743,0.0002717139,0.000025967198,0.00009962412,0.00009038101,0.000044786328],"domain_scores_gemma":[0.9965384,0.0019655442,0.00040106982,0.0003865922,0.00049803016,0.00021047398],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018274933,0.0005804656,0.00038194912,0.0032281117,0.00066900835,0.00060667243,0.00065091765,0.0004613523,0.0007081247],"category_scores_gemma":[0.007473019,0.00021600668,0.0007886551,0.0013086855,0.0007348603,0.00049690076,0.0010561409,0.0005278672,0.0001332546],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007770397,0.0002297395,0.41592976,0.00037123734,0.0007010522,0.00056768797,0.0015163993,0.32056096,0.025945924,0.013451245,0.0025325352,0.21741632],"study_design_scores_gemma":[0.000016742493,0.000041368614,0.0792879,0.000014284958,0.000028354409,0.00007362301,0.00019312541,0.910797,0.001380552,0.007669751,0.0004619065,0.000035371195],"about_ca_topic_score_codex":0.0135974465,"about_ca_topic_score_gemma":0.010237295,"teacher_disagreement_score":0.0135974465,"about_ca_system_score_codex":0.00077853916,"about_ca_system_score_gemma":0.00065194356,"threshold_uncertainty_score":0.027036607},"labels":[],"label_agreement":null},{"id":"W3199755963","doi":"10.3847/1538-4357/ac2b9f","title":"Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent Galaxies","year":2022,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Universidad Andrés Bello; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Star formation; Star (game theory); Stellar mass","score_opus":0.006888120327645898,"score_gpt":0.2103661509880972,"score_spread":0.20347803066045128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199755963","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9919326,0.0005396605,0.0014509034,0.00027575417,0.00005122721,0.00002653798,0.0008845745,0.00031376697,0.0045249783],"genre_scores_gemma":[0.9979119,0.00004166712,0.00074795424,0.0001523437,0.000022876553,0.0000055630862,0.00042538904,0.00003059359,0.0006618174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980944,0.000008145179,0.000008831312,0.00006292406,0.00006104511,0.00004966256],"domain_scores_gemma":[0.9993407,0.000052375057,0.00019018122,0.00010656689,0.00006990441,0.00024028416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003086831,0.0003496399,0.00033071724,0.0008357183,0.0008978773,0.00083061197,0.00073312176,0.000533775,0.0020634672],"category_scores_gemma":[0.0005295055,0.00025197043,0.00030245967,0.0005133105,0.0005304208,0.00027948685,0.00092494016,0.0004850934,0.0011488491],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041120002,0.000096327545,0.60791576,0.000081420825,0.00013532433,0.0052665733,0.0010425801,0.000245324,0.36340764,0.001687724,0.0037323202,0.015977686],"study_design_scores_gemma":[0.000027509555,0.00023488907,0.95328665,0.00002022295,0.00009509546,0.0041704806,0.00033336983,0.0011092263,0.02811399,0.000674269,0.011908402,0.000025751195],"about_ca_topic_score_codex":0.004039921,"about_ca_topic_score_gemma":0.004605096,"teacher_disagreement_score":0.004039921,"about_ca_system_score_codex":0.0006926612,"about_ca_system_score_gemma":0.00021089452,"threshold_uncertainty_score":0.008032799},"labels":[],"label_agreement":null},{"id":"W3199912069","doi":"10.3847/1538-4357/ac1f2d","title":"Erratum: “Searches for Continuous Gravitational Waves from Nine Young Supernova Remnants” (2015, ApJ, 813, 39) <sup>*</sup>","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Physics; Supernova; Gravitational wave; Astronomy; Astrophysics","score_opus":0.020838697617548634,"score_gpt":0.31537341721339457,"score_spread":0.29453471959584593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199912069","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0031639826,0.0021165903,0.002620766,0.048128217,0.91882557,0.00003572933,0.0062117353,0.0014187758,0.017478598],"genre_scores_gemma":[0.08694627,0.013336891,0.025489433,0.11124605,0.20356543,0.0002573864,0.048761535,0.008854419,0.50154257],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9982444,0.00016531759,0.00037876776,0.00026989117,0.00083400344,0.000107619664],"domain_scores_gemma":[0.991117,0.0018242567,0.0009569316,0.0008964777,0.004761925,0.00044348423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015351269,0.0017824831,0.0010169051,0.00317452,0.0034398148,0.0034702453,0.0019949025,0.0029937327,0.039639458],"category_scores_gemma":[0.020096404,0.00093748566,0.0011773956,0.002840278,0.0016043573,0.0022226486,0.0018991214,0.005916524,0.034726422],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046298308,0.000013911616,0.00061556324,0.00007676189,0.000018106313,0.00015412398,0.000050131206,0.00006607369,0.00016252909,0.0011743141,0.9893085,0.00831364],"study_design_scores_gemma":[0.000041846295,0.000040432456,0.008166919,0.00037629233,0.00008671655,0.0009656666,0.0003505288,0.00036751537,0.001641155,0.0031046057,0.9847777,0.00008058857],"about_ca_topic_score_codex":0.015459938,"about_ca_topic_score_gemma":0.020864632,"teacher_disagreement_score":0.039639458,"about_ca_system_score_codex":0.0024792925,"about_ca_system_score_gemma":0.0023828605,"threshold_uncertainty_score":0.13260716},"labels":[],"label_agreement":null},{"id":"W3199983395","doi":"10.3847/1538-4357/ac0ce9","title":"The JCMT BISTRO Survey: An 850/450 μm Polarization Study of NGC 2071IR in Orion B","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; University of Manitoba; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics; McMaster University; Queen's University","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Polarization (electrochemistry); James Clerk Maxwell Telescope; Magnetic field; Sky; Outflow; Stars; Brewster's angle; Young stellar object; Star formation; Optics","score_opus":0.0171233694113493,"score_gpt":0.2690159077526851,"score_spread":0.2518925383413358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3199983395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988564,0.000032848624,0.00005930983,0.000016337774,0.0000015194526,0.000003863218,0.00048592238,0.000016704043,0.0005270067],"genre_scores_gemma":[0.9974317,0.00004614265,0.00031784578,0.000027951883,0.000011399561,0.000008333132,0.0019034253,0.00001223356,0.00024103512],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998202,0.000016980468,0.000007941958,0.00004901752,0.000053454274,0.000052422274],"domain_scores_gemma":[0.9994999,0.000034312616,0.00014629422,0.00004826282,0.000092482696,0.00017873372],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020339963,0.00021244207,0.00023340563,0.0015810431,0.00045733774,0.00042012983,0.00027735397,0.00028513055,0.000739567],"category_scores_gemma":[0.00034725593,0.00015423787,0.00016537485,0.0008735604,0.00019610673,0.00017430882,0.00045996203,0.00020547931,0.00031538936],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016012529,0.000106714455,0.9506583,0.000026245696,0.000051220468,0.00049485575,0.0005373542,0.00020528868,0.036468845,0.00006827472,0.0008589566,0.010363767],"study_design_scores_gemma":[0.0000018887449,0.000008762425,0.9991153,0.0000016653752,0.000004907495,0.00007935629,0.00007936008,0.00014221689,0.00033658108,0.0000034465834,0.0002247443,0.0000018586222],"about_ca_topic_score_codex":0.014425172,"about_ca_topic_score_gemma":0.023652447,"teacher_disagreement_score":0.014425172,"about_ca_system_score_codex":0.00030512194,"about_ca_system_score_gemma":0.00022342766,"threshold_uncertainty_score":0.02868241},"labels":[],"label_agreement":null},{"id":"W3200005856","doi":"10.3847/1538-4357/ac1f96","title":"On the Three-dimensional Structure of Local Molecular Clouds","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":90,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of Alberta","funders":"","keywords":"Molecular cloud; Extinction (optical mineralogy); Gaussian; Interstellar cloud; Sky; Envelope (radar); Protostar","score_opus":0.006518689068631144,"score_gpt":0.21823839210652848,"score_spread":0.21171970303789733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3200005856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97650164,0.00018445861,0.020177068,0.00019419717,0.000010326001,0.000024765994,0.0006911837,0.0004150422,0.0018012972],"genre_scores_gemma":[0.9916671,0.000085389904,0.0075273225,0.000028769267,0.000009067608,0.000009572125,0.00051709305,0.000046297642,0.0001094128],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99992657,0.000010563638,0.0000030216186,0.000020741345,0.00002298092,0.000016140408],"domain_scores_gemma":[0.9995689,0.000087259206,0.000100854464,0.00006979565,0.00011684826,0.000056375164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014065168,0.00017649202,0.000244744,0.0012900266,0.0004397115,0.0010513444,0.00038271982,0.00023091212,0.0012107954],"category_scores_gemma":[0.0012728731,0.00023303363,0.0003452287,0.0008095487,0.0004671238,0.00047958217,0.0008322666,0.00034424715,0.0002619557],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039008696,0.00021166097,0.20881262,0.00020186123,0.0003256884,0.0010567558,0.0012063816,0.61656696,0.07979128,0.015819835,0.0031929677,0.072423816],"study_design_scores_gemma":[0.000026596968,0.0000322606,0.13154162,0.000034418543,0.000030102092,0.00021238133,0.00025759265,0.854788,0.004762834,0.006058201,0.0022077565,0.00004825164],"about_ca_topic_score_codex":0.008422391,"about_ca_topic_score_gemma":0.008161484,"teacher_disagreement_score":0.008422391,"about_ca_system_score_codex":0.0006551398,"about_ca_system_score_gemma":0.00039384168,"threshold_uncertainty_score":0.01674676},"labels":[],"label_agreement":null},{"id":"W3200244874","doi":"10.3847/1538-4357/ac7dab","title":"Tidal Distortions in NGC1052-DF2 and NGC1052-DF4: Independent Evidence for a Lack of Dark Matter","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Dark matter; Dark galaxy; Elliptical galaxy; Dark matter halo; Galaxy; Galaxy group; Astronomy; Cuspy halo problem; Surface brightness; Fundamental plane (elliptical galaxies); Halo; Lenticular galaxy","score_opus":0.024711441871692417,"score_gpt":0.26832357136690366,"score_spread":0.24361212949521124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3200244874","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99805707,0.000046733214,0.00016100425,0.000014344954,0.000002731789,0.0000038553503,0.00014058276,0.000025249177,0.0015483666],"genre_scores_gemma":[0.99917895,0.000008475962,0.00014709293,0.000011330262,0.000004273104,0.000003035383,0.00042482532,0.000005610176,0.00021627692],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997315,0.000017559347,0.000018673263,0.00007146918,0.000082044506,0.00007882314],"domain_scores_gemma":[0.9991073,0.00006343459,0.0002894927,0.00013352303,0.0000998968,0.0003061945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023673342,0.0004159981,0.00031170636,0.0024205856,0.00058652856,0.0007793657,0.00044007043,0.00047447375,0.0023436763],"category_scores_gemma":[0.0004911646,0.00023785811,0.00031047166,0.0008401021,0.00053170754,0.00028250233,0.0008230308,0.00027701413,0.00048698435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003121877,0.00007500626,0.9290029,0.000034747518,0.00012119311,0.00054696883,0.00052872614,0.00023590078,0.06288992,0.00023785529,0.00038174947,0.0056328867],"study_design_scores_gemma":[0.0000073226715,0.000039562437,0.99789184,0.0000028973811,0.000013049916,0.00025011314,0.00021707422,0.00016528348,0.0009518004,0.000036330646,0.00042027494,0.000004442789],"about_ca_topic_score_codex":0.005035296,"about_ca_topic_score_gemma":0.0077599455,"teacher_disagreement_score":0.005035296,"about_ca_system_score_codex":0.00043747344,"about_ca_system_score_gemma":0.00011343042,"threshold_uncertainty_score":0.010011971},"labels":[],"label_agreement":null},{"id":"W3200736299","doi":"10.3847/1538-4357/ac510d","title":"Search for Lensing Signatures from the Latest Fast Radio Burst Observations and Constraints on the Abundance of Primordial Black Holes","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Natural Science Foundation of China","keywords":"Physics; Primordial black hole; Astrophysics; Dark matter; Monochromatic color; Millisecond; Gravitational wave; Binary black hole; Gravitational lens; Flux (metallurgy); Astronomy; Redshift; Galaxy; Optics","score_opus":0.031471844110136225,"score_gpt":0.3012563881776639,"score_spread":0.2697845440675277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3200736299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99157965,0.00025116824,0.0056319064,0.000051636416,0.0000026776218,0.000009101462,0.0010098332,0.00007998627,0.0013840119],"genre_scores_gemma":[0.9956391,0.000069425376,0.0026269932,0.000009338797,0.000007777116,0.0000038758535,0.0014933993,0.000007476669,0.00014255449],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954,0.000059257152,0.000026184594,0.00010210303,0.00016415768,0.00010827946],"domain_scores_gemma":[0.99790823,0.0005949012,0.0007550517,0.00021155835,0.0002781553,0.00025213038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001039526,0.00035820695,0.00034939064,0.00288911,0.0003733727,0.0007389333,0.00041339826,0.00031783347,0.0012549948],"category_scores_gemma":[0.0026846908,0.00018668623,0.0003661165,0.0014055845,0.00026577682,0.00042636067,0.0005789961,0.00018349513,0.00021587736],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012536801,0.00002552046,0.96684104,0.0000436775,0.00008405941,0.00017132884,0.000057254314,0.0024203223,0.013905438,0.00086318096,0.0004016324,0.015061102],"study_design_scores_gemma":[0.000010557237,0.000031247084,0.9607184,0.000015700129,0.00005047078,0.00019907854,0.00011882852,0.02994599,0.0073143756,0.00060437876,0.0009761433,0.00001479081],"about_ca_topic_score_codex":0.02074045,"about_ca_topic_score_gemma":0.02985051,"teacher_disagreement_score":0.02074045,"about_ca_system_score_codex":0.0005844644,"about_ca_system_score_gemma":0.0006709928,"threshold_uncertainty_score":0.04123944},"labels":[],"label_agreement":null},{"id":"W3200913255","doi":"10.3847/1538-4357/ac28a1","title":"Magnetic Fields in Massive Star-forming Regions (MagMaR). II. Tomography through Dust and Molecular Line Polarization in NGC 6334I(N)","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Alberta Livestock and Meat Agency; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Astronomy; Interstellar medium; Star formation; Magnetic field; Line (geometry); Stars; Galaxy","score_opus":0.007799258779127665,"score_gpt":0.22846762404850374,"score_spread":0.22066836526937608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3200913255","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99946016,0.000025640778,0.00010234366,0.000013015869,7.028632e-7,0.0000018342201,0.00007361457,0.000013160695,0.00030952247],"genre_scores_gemma":[0.99964,0.000012107605,0.00018080624,0.000005850138,0.000002032921,0.0000011067948,0.00008015153,0.0000022293846,0.000075679025],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999652,0.0000042973247,0.0000013208542,0.000009379778,0.0000077408085,0.0000120334835],"domain_scores_gemma":[0.9998989,0.000008697927,0.00004147104,0.000008693465,0.000013936452,0.000028292821],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009147166,0.00012971256,0.00008177977,0.0005118489,0.00019838687,0.00018553066,0.00016492291,0.00014435328,0.00051284756],"category_scores_gemma":[0.00024810186,0.00010065092,0.00009337306,0.00020253129,0.0001492162,0.000106797495,0.00024573776,0.00013483144,0.00016942239],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017426263,0.00002897425,0.85853535,0.000013690776,0.000024366791,0.00064341706,0.00047092326,0.0005925921,0.12951143,0.000109811146,0.0003328604,0.009562388],"study_design_scores_gemma":[0.0000026011837,0.000019334459,0.99822766,0.0000013217126,0.000004663263,0.00017939569,0.000078933765,0.00041999941,0.0007813508,0.000032820368,0.00025041477,0.0000016504465],"about_ca_topic_score_codex":0.009998399,"about_ca_topic_score_gemma":0.016589444,"teacher_disagreement_score":0.009998399,"about_ca_system_score_codex":0.0002439305,"about_ca_system_score_gemma":0.000067169705,"threshold_uncertainty_score":0.019880414},"labels":[],"label_agreement":null},{"id":"W3201114642","doi":"10.3847/1538-4357/ac350f","title":"SNEWPY: A Data Pipeline from Supernova Simulations to Neutrino Signals","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Laurentian University","funders":"Vetenskapsrådet; U.S. Department of Energy; Science and Technology Facilities Council; National Science Foundation","keywords":"Neutrino; Supernova; Physics; Neutrino detector; Detector; Event (particle physics); Astrophysics; Neutrino oscillation; Nuclear physics","score_opus":0.05497565888542118,"score_gpt":0.33128583719842125,"score_spread":0.2763101783130001,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3201114642","genre_codex":"software","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.004824281,0.00020460133,0.19374627,0.00031356572,0.00020874143,0.00029927475,0.038333397,0.75808066,0.0039892565],"genre_scores_gemma":[0.1181614,0.0009107686,0.30445692,0.0014395163,0.00029304568,0.0030995435,0.25840348,0.30098972,0.012245549],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9982948,0.00025881472,0.00019396699,0.000455066,0.00064729573,0.00015008746],"domain_scores_gemma":[0.9960168,0.0014381215,0.00028734276,0.0010753163,0.0007802789,0.0004021058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028935445,0.004097901,0.001994541,0.003030574,0.000958095,0.003145652,0.004911349,0.0012282524,0.039019413],"category_scores_gemma":[0.010812408,0.0026646992,0.0033044459,0.0024672763,0.0011097112,0.0036896982,0.005530757,0.00397454,0.022211822],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028945997,0.00044330774,0.012933484,0.0023323023,0.0012197354,0.0012419878,0.0012457226,0.072547406,0.020609602,0.026483284,0.6802139,0.17783454],"study_design_scores_gemma":[0.0017624887,0.00024408502,0.0075703636,0.0002929962,0.00020775727,0.00036464728,0.00016215976,0.44800898,0.06284515,0.05970211,0.41822404,0.00061516336],"about_ca_topic_score_codex":0.0065010255,"about_ca_topic_score_gemma":0.0046065054,"teacher_disagreement_score":0.039019413,"about_ca_system_score_codex":0.0014116479,"about_ca_system_score_gemma":0.002767626,"threshold_uncertainty_score":0.13053292},"labels":[],"label_agreement":null},{"id":"W3201312629","doi":"10.3847/1538-4357/ac1f2c","title":"Erratum: “Searches for Continuous Gravitational Waves from 15 Supernova Remnants and Fomalhaut b with Advanced LIGO” (2019, ApJ, 875, 122) <sup>*</sup>","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Johns Hopkins University; University of Pennsylvania","keywords":"LIGO; Supernova; Gravitational wave; Physics; Astrophysics; Astronomy","score_opus":0.013724562396540935,"score_gpt":0.2919306741001394,"score_spread":0.27820611170359844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3201312629","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0009466268,0.0015755869,0.0006930377,0.052839044,0.9215494,0.000020540492,0.0052033653,0.0007079121,0.016464535],"genre_scores_gemma":[0.02986609,0.006560101,0.0073642423,0.11428291,0.23861481,0.00020060637,0.028090887,0.0041454076,0.570875],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9980317,0.00021736712,0.00045931607,0.0002733854,0.0008961415,0.00012214338],"domain_scores_gemma":[0.9876481,0.002875778,0.001095679,0.00092569744,0.006751808,0.0007029164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020854136,0.00204047,0.0012226659,0.0033251573,0.0040475433,0.0055030542,0.0016453891,0.0034808961,0.052289706],"category_scores_gemma":[0.023392782,0.000884049,0.0010990844,0.0026526242,0.0015730903,0.0026226842,0.0020314278,0.0062869936,0.060462613],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000038717495,0.000009659899,0.00022329582,0.000042028525,0.000007578027,0.00006502476,0.000019319825,0.00002427801,0.000043983855,0.0009139862,0.9943634,0.0042486372],"study_design_scores_gemma":[0.000052242267,0.00004052847,0.006064479,0.00034463918,0.000063162166,0.00044331158,0.0002239808,0.00028648617,0.0007529755,0.0032543251,0.9884077,0.00006622741],"about_ca_topic_score_codex":0.022250535,"about_ca_topic_score_gemma":0.029933602,"teacher_disagreement_score":0.052289706,"about_ca_system_score_codex":0.0028320476,"about_ca_system_score_gemma":0.0032143109,"threshold_uncertainty_score":0.17492652},"labels":[],"label_agreement":null},{"id":"W3201425423","doi":"10.3847/1538-4357/ac4bc7","title":"A Sudden Period of High Activity from Repeating Fast Radio Burst 20201124A","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":77,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; University of Toronto; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Research Chairs; National Defense Science and Engineering Graduate; Smithsonian Astrophysical Observatory; U.S. Department of Defense; Gordon and Betty Moore Foundation; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Physics; Period (music); Astrophysics; Astronomy; Acoustics","score_opus":0.009108045211027182,"score_gpt":0.21493906569621735,"score_spread":0.20583102048519017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3201425423","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.994284,0.00022266875,0.0013193461,0.00018052742,0.00003891106,0.000016229811,0.0009678776,0.00029648634,0.0026740287],"genre_scores_gemma":[0.9968077,0.00004086538,0.00085935957,0.00005673001,0.000035366713,0.0000108957665,0.0013979306,0.000051048853,0.00074007135],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998735,0.00001095264,0.000005340121,0.000034086264,0.000045849978,0.000030227051],"domain_scores_gemma":[0.9995784,0.00007843624,0.00011396614,0.000048045527,0.00005306968,0.00012817286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024311831,0.00032930588,0.0003176269,0.0007836534,0.0005380605,0.0006147218,0.0003344035,0.0005162868,0.0019971195],"category_scores_gemma":[0.00084406714,0.00017360107,0.00028841777,0.00044023365,0.00025678967,0.00017215985,0.0004347306,0.0005565767,0.0007198495],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010811342,0.00020894242,0.7280283,0.0001921405,0.00030559365,0.010548201,0.0011190209,0.006421427,0.17613441,0.0012023371,0.012529953,0.06222847],"study_design_scores_gemma":[0.000019958177,0.00012138661,0.98357046,0.000021331958,0.000037767564,0.0018412166,0.00012877242,0.0037667912,0.005543931,0.00019693113,0.004719699,0.000031823653],"about_ca_topic_score_codex":0.004793795,"about_ca_topic_score_gemma":0.00621221,"teacher_disagreement_score":0.004793795,"about_ca_system_score_codex":0.00042927536,"about_ca_system_score_gemma":0.0001402515,"threshold_uncertainty_score":0.009531796},"labels":[],"label_agreement":null},{"id":"W3201625252","doi":"10.3847/1538-4357/ac2901","title":"An IFU View of the Active Galactic Nuclei in MaNGA Galaxy Pairs","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Social Science Fund of China; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Chinese Academy of Sciences; University of Oxford; York University; Chinese Academy of Sciences South America Center for Astronomy; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Astronomy; Star formation; Balmer series; Galaxy formation and evolution; Surface brightness; Emission spectrum; Spectral line","score_opus":0.008048400706680182,"score_gpt":0.22167115434268087,"score_spread":0.2136227536360007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3201625252","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99716896,0.00023458387,0.00015544535,0.000032807802,0.0000040625528,0.000003873913,0.00029415722,0.000012136571,0.002093996],"genre_scores_gemma":[0.99953675,0.000020449892,0.00009632702,0.0000063881416,0.000004170312,0.0000019739928,0.00014372532,0.000001956686,0.00018823743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998228,0.000034465138,0.000006486748,0.000053060692,0.00001945337,0.00006386049],"domain_scores_gemma":[0.99961793,0.000057463905,0.000112383284,0.00003065221,0.0000420051,0.00013956334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018297083,0.00014790699,0.00019753842,0.0024892786,0.00070329616,0.00056826195,0.00016684103,0.00022632362,0.0025816222],"category_scores_gemma":[0.00050555076,0.00010635572,0.00018659563,0.0009743395,0.00026372616,0.00025526987,0.0006131781,0.0001138691,0.0004423829],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000057302917,0.000015088318,0.9923131,0.000007958366,0.000019119643,0.00021763833,0.00027384947,0.000082940576,0.0037484209,0.0001333562,0.0001799556,0.0029512674],"study_design_scores_gemma":[6.0445194e-7,0.000014735591,0.9986766,0.0000022477611,0.0000054601305,0.00022191051,0.00027332763,0.00028307855,0.00019018866,0.00004293828,0.00028762937,0.0000013023196],"about_ca_topic_score_codex":0.009430551,"about_ca_topic_score_gemma":0.013393694,"teacher_disagreement_score":0.009430551,"about_ca_system_score_codex":0.0003466014,"about_ca_system_score_gemma":0.00011725015,"threshold_uncertainty_score":0.018751323},"labels":[],"label_agreement":null},{"id":"W3201814109","doi":"10.3847/1538-4357/ac2fa7","title":"Types of Transients in the Centers of Post-starburst and Quiescent Balmer-strong Galaxies","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Physics; Galaxy; Astrophysics; Balmer series; Supernova; Active galactic nucleus; Astronomy; Light curve; Emission spectrum; Spectral line","score_opus":0.011863571035599176,"score_gpt":0.2373910647248333,"score_spread":0.2255274936892341,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3201814109","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99431616,0.000218773,0.0003275982,0.000039566363,0.0000043484847,0.000012446107,0.002933498,0.00010469789,0.0020429513],"genre_scores_gemma":[0.9934889,0.00010031741,0.0003419292,0.000028794975,0.000010660708,0.000007103343,0.005332543,0.00001400399,0.00067572144],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970275,0.000018928433,0.000031146905,0.00008173844,0.000073235766,0.00009213416],"domain_scores_gemma":[0.99758124,0.00030971493,0.001193712,0.00024056529,0.00031386522,0.00036091506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000407264,0.00015568487,0.00021148977,0.0041194316,0.00037987457,0.0008693206,0.00032846179,0.00025544566,0.0038218724],"category_scores_gemma":[0.0015275024,0.00009675214,0.00025726753,0.0018156059,0.00028344605,0.00053814054,0.0006143885,0.0001507155,0.00083731697],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048724658,0.000023012804,0.98664874,0.000022589315,0.000018367173,0.00008511803,0.000313263,0.00009139203,0.002271354,0.00017627669,0.0010029332,0.009298249],"study_design_scores_gemma":[0.0000021387875,0.000012791573,0.9983541,0.000007013075,0.000006815142,0.00015320368,0.00014844903,0.00014551877,0.0003042568,0.000036326477,0.00082677335,0.0000027131498],"about_ca_topic_score_codex":0.012668487,"about_ca_topic_score_gemma":0.013592363,"teacher_disagreement_score":0.012668487,"about_ca_system_score_codex":0.00039552184,"about_ca_system_score_gemma":0.00021968782,"threshold_uncertainty_score":0.025189519},"labels":[],"label_agreement":null},{"id":"W3201831329","doi":"10.3847/1538-4357/ac2b29","title":"The EDGE-CALIFA Survey: The Resolved Star Formation Efficiency and Local Physical Conditions","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Star formation; RADIUS; Galaxy; Star (game theory); Stellar mass; Flattening; Metallicity; Sigma; Quantum mechanics","score_opus":0.014505473566367274,"score_gpt":0.25499900503668715,"score_spread":0.24049353147031988,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3201831329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974482,0.000052853662,0.000033975706,0.00001364041,7.6397015e-7,0.0000027449064,0.0011237155,0.0000054738657,0.0013187218],"genre_scores_gemma":[0.99715436,0.000051085994,0.000102356265,0.000012997759,0.000004310001,0.000004456571,0.0021785581,0.0000036293914,0.00048830116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979895,0.000027439564,0.000009577535,0.000084123276,0.00004716238,0.00003277137],"domain_scores_gemma":[0.99867994,0.00019828226,0.00037944617,0.00015969301,0.00028805743,0.00029450687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030234494,0.0001482347,0.0002244703,0.000987505,0.00029522073,0.00070564635,0.00030177415,0.00018966821,0.0018989027],"category_scores_gemma":[0.000715287,0.00014453386,0.00010908067,0.0008696048,0.00023081197,0.00022533104,0.00043555812,0.00018125626,0.00039302593],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050994033,0.000007546178,0.9983083,0.0000034381258,0.000015074957,0.000020266314,0.000044214987,0.000040713338,0.00046281703,0.000016926422,0.00015616485,0.00087352743],"study_design_scores_gemma":[0.0000017478715,0.000004734697,0.99966514,0.0000020054626,0.0000033821127,0.000019130244,0.000044531105,0.00007718641,0.000048836722,0.0000026252999,0.00012973901,8.6713925e-7],"about_ca_topic_score_codex":0.078623295,"about_ca_topic_score_gemma":0.17786385,"teacher_disagreement_score":0.078623295,"about_ca_system_score_codex":0.00047336475,"about_ca_system_score_gemma":0.00020551283,"threshold_uncertainty_score":0.1563313},"labels":[],"label_agreement":null},{"id":"W3201947131","doi":"10.3847/1538-4357/ac2c66","title":"A Machine-learning Approach to Integral Field Unit Spectroscopy Observations. III. Disentangling Multiple Components in H ii Regions","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Chemometric Analyses","field":"Chemistry","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; Institut de Valorisation des Données; Fonds de recherche du Québec – Nature et technologies; Université de Montréal; Institut national des sciences de l'Univers; Fundação de Amparo à Pesquisa e Inovação do Estado de Santa Catarina; Centre National de la Recherche Scientifique; Conselho Nacional de Desenvolvimento Científico e Tecnológico","keywords":"Artificial intelligence; Artificial neural network; Convolutional neural network; Computer science; Spectral line; Filter (signal processing); Pattern recognition (psychology); Component (thermodynamics); Line (geometry); Kinematics; Telescope; Inference; Physics; Segmentation; Galaxy; Astrophysics; Computer vision; Mathematics; Astronomy; Geometry","score_opus":0.04800305053096856,"score_gpt":0.2774129259861079,"score_spread":0.22940987545513933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3201947131","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.34671387,0.0006946428,0.6455568,0.00054591184,0.000039457907,0.00006875324,0.0003357675,0.00057445833,0.0054703057],"genre_scores_gemma":[0.85802156,0.00013399248,0.13990128,0.000053639353,0.000050758135,0.000029757384,0.00021205291,0.000039848386,0.0015572228],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998648,0.00004517966,0.0000044413573,0.00004294225,0.000028535951,0.000014118294],"domain_scores_gemma":[0.9997658,0.000100368816,0.00005075023,0.000029772646,0.000039448667,0.0000138030355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006451289,0.0002761969,0.00017822236,0.00072712335,0.00032409735,0.00053283357,0.00056893425,0.00042913665,0.00076451234],"category_scores_gemma":[0.0013596656,0.00023305784,0.00032875314,0.000595116,0.0002921255,0.0005620985,0.00037860882,0.00049551704,0.00014565687],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014126975,0.0002042743,0.028066393,0.00007492855,0.00015053526,0.000100013545,0.000116818235,0.647209,0.030915517,0.013596713,0.0015864515,0.27783808],"study_design_scores_gemma":[0.000002668932,0.000009659012,0.005267193,0.0000026145708,0.000003804984,0.000012697366,0.000010927092,0.989819,0.0014898251,0.003005424,0.00037056522,0.000005632139],"about_ca_topic_score_codex":0.007869772,"about_ca_topic_score_gemma":0.014671613,"teacher_disagreement_score":0.007869772,"about_ca_system_score_codex":0.0008554232,"about_ca_system_score_gemma":0.0002642759,"threshold_uncertainty_score":0.015647948},"labels":[],"label_agreement":null},{"id":"W3202182240","doi":"10.3847/1538-4357/ac2c6b","title":"The MAVERIC Survey: Variable Jet-accretion Coupling in Luminous Accreting Neutron Stars in Galactic Globular Clusters","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Science Foundation","keywords":"Physics; Neutron star; Astrophysics; Globular cluster; Accretion (finance); Astronomy; Luminosity; X-ray burster; Black hole (networking); X-ray binary; Compact star; Stars; Galaxy; Stellar evolution; Stellar mass loss","score_opus":0.014706372775186641,"score_gpt":0.23637484662162767,"score_spread":0.22166847384644103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3202182240","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99957436,0.000053677213,0.000023626659,0.000004683237,5.473919e-7,0.0000016354234,0.0001581421,0.0000034438228,0.00017997329],"genre_scores_gemma":[0.9991697,0.00005012491,0.00008844059,0.000008417065,0.0000024744638,0.0000022746337,0.0005939141,0.0000021006852,0.00008252977],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997241,0.000041899293,0.00002610379,0.00010219959,0.00004643591,0.000059261678],"domain_scores_gemma":[0.99899405,0.000107363194,0.00036155118,0.000115217954,0.00011851822,0.0003033615],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038971752,0.00025324375,0.00027240385,0.0022808383,0.00046470005,0.0006685494,0.0003492789,0.000259425,0.00045953516],"category_scores_gemma":[0.00069071323,0.00014512741,0.00014754695,0.0014614975,0.0003120358,0.00022919662,0.000914212,0.00014226952,0.00014650922],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029522571,0.000010450257,0.996329,0.000005137578,0.000019257384,0.000038458118,0.00014790327,0.000053640884,0.0021211284,0.000025463496,0.00005467528,0.0011653787],"study_design_scores_gemma":[9.2730556e-7,0.000010118671,0.99961483,9.935766e-7,0.0000039028105,0.00004787735,0.00008107465,0.00005076944,0.00008144794,0.0000033526555,0.00010405872,7.3323594e-7],"about_ca_topic_score_codex":0.012060584,"about_ca_topic_score_gemma":0.02949845,"teacher_disagreement_score":0.012060584,"about_ca_system_score_codex":0.00038398063,"about_ca_system_score_gemma":0.00026667077,"threshold_uncertainty_score":0.023980737},"labels":[],"label_agreement":null},{"id":"W3202256392","doi":"10.3847/1538-4357/ac5f57","title":"The Criterion for Chaos in Three-planet Systems","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Quantum chaos and dynamical systems","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Planet; Chaotic; Statistical physics; Interplanetary spaceflight; CHAOS (operating system); Classical mechanics; Astrophysics; Asteroid; Work (physics); Lyapunov exponent; Nonlinear system; Computer science; Quantum mechanics; Astronomy; Solar wind","score_opus":0.01007086733991448,"score_gpt":0.2309266395470819,"score_spread":0.22085577220716743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3202256392","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.67990047,0.00060990907,0.29044327,0.0007788378,0.000070265036,0.000092608345,0.00026191055,0.00036929495,0.027473394],"genre_scores_gemma":[0.98629063,0.0000532146,0.012885071,0.0000294848,0.000018900311,0.00004515618,0.000060096696,0.000038919563,0.00057863694],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99934655,0.00014881472,0.00004506899,0.00009931707,0.00026375888,0.00009652652],"domain_scores_gemma":[0.9961791,0.0018960559,0.00044557083,0.00034834348,0.000773327,0.0003576184],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010982853,0.00025015217,0.00066334923,0.0013117946,0.0010670607,0.000979159,0.00061162526,0.0006428852,0.0020788012],"category_scores_gemma":[0.0075278645,0.00018183373,0.00041836197,0.00035492377,0.0019896887,0.0014267775,0.0015807856,0.00077531935,0.00033862432],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012823119,0.000031760334,0.008941144,0.00018386023,0.00005225823,0.00040665033,0.00051317253,0.19847648,0.024222929,0.75342417,0.0015574526,0.012061869],"study_design_scores_gemma":[0.000022569733,0.00007342258,0.00537291,0.000048169062,0.000008843511,0.00022724342,0.00011755945,0.7324461,0.00605337,0.25279143,0.0027912222,0.000047278812],"about_ca_topic_score_codex":0.0011663529,"about_ca_topic_score_gemma":0.0005974427,"teacher_disagreement_score":0.0020788012,"about_ca_system_score_codex":0.0008619361,"about_ca_system_score_gemma":0.0006345674,"threshold_uncertainty_score":0.0069543123},"labels":[],"label_agreement":null},{"id":"W3202363815","doi":"10.3847/1538-4357/ac2c6a","title":"Multiwavelength Observation Campaign of the TeV Gamma-Ray Binary HESS J0632 + 057 with NuSTAR, VERITAS, MDM, and Swift","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; McGill University","funders":"Jet Propulsion Laboratory; National Research Foundation; Dartmouth College; National Energy Research Scientific Computing Center; Ohio State University; Office of Science; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; National Research Foundation of Korea; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Science Foundation","keywords":"Physics; Swift; Astrophysics; Binary number; Astronomy; Gamma ray","score_opus":0.008941981785897753,"score_gpt":0.19947274189554653,"score_spread":0.19053076010964878,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3202363815","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843043,0.00003722406,0.00009947806,0.000012946073,0.0000052127593,0.0000059561053,0.0009932528,0.000025896481,0.00038956504],"genre_scores_gemma":[0.9946549,0.000022116035,0.0007423772,0.000013198344,0.000012254786,0.000009512288,0.0042629493,0.000008360872,0.0002743756],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979347,0.000023724173,0.000012772261,0.00007579957,0.000055911038,0.000038408554],"domain_scores_gemma":[0.9995763,0.000035865818,0.00012719842,0.00006207071,0.000069802954,0.00012881665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034541846,0.00021147766,0.00023564325,0.0008942406,0.00034129148,0.0003186341,0.0002431721,0.00025308205,0.0006154308],"category_scores_gemma":[0.00036065193,0.00015008148,0.00017560822,0.0006948757,0.00014015258,0.00021937804,0.000521466,0.0002033816,0.00026281102],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006195507,0.0002184481,0.93228716,0.000058262794,0.00013047902,0.0007611518,0.00044911192,0.0015697364,0.043669835,0.00020968377,0.0018595217,0.01816703],"study_design_scores_gemma":[0.000019295809,0.00011427467,0.9937091,0.000007078035,0.00002306586,0.00020901035,0.00015474741,0.0022077009,0.0020674851,0.000026029064,0.0014538534,0.00000841179],"about_ca_topic_score_codex":0.008429083,"about_ca_topic_score_gemma":0.023133814,"teacher_disagreement_score":0.008429083,"about_ca_system_score_codex":0.00028806654,"about_ca_system_score_gemma":0.00027808108,"threshold_uncertainty_score":0.016760051},"labels":[],"label_agreement":null},{"id":"W3203283734","doi":"10.3847/1538-4357/ac2b9e","title":"Multiphase Outflows in High-redshift Quasar Host Galaxies","year":2021,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Quasar; Galaxy; Star formation; Astronomy; Redshift; Luminosity; Interstellar medium; Dark galaxy; Galaxy formation and evolution; Galaxy merger","score_opus":0.01397121287163109,"score_gpt":0.25495710944506833,"score_spread":0.24098589657343725,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3203283734","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939454,0.00005515507,0.00026223477,0.000008657739,0.0000011569441,0.0000019815861,0.000050197188,0.000019197596,0.00020693836],"genre_scores_gemma":[0.9997545,0.000011782843,0.00010981535,0.000004497223,0.0000041316252,0.0000013003861,0.00007662378,0.0000012982537,0.000036154423],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988186,0.000016273036,0.0000075826197,0.000029100824,0.00002923911,0.00003593112],"domain_scores_gemma":[0.9988587,0.00018804752,0.00054602465,0.0000726261,0.00009267156,0.00024194967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033224362,0.00018308076,0.00016990691,0.0010796717,0.00027072194,0.0006227113,0.00025307768,0.00024642848,0.00093986065],"category_scores_gemma":[0.00059946754,0.00016356418,0.00016075782,0.00041571408,0.00020606497,0.00029616148,0.00047736624,0.0002071751,0.00010970111],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056774217,0.000039946794,0.9768435,0.00001085782,0.000029689674,0.00014208432,0.00015288177,0.00033171853,0.019549098,0.0001335594,0.00006031458,0.0026495717],"study_design_scores_gemma":[0.0000031617794,0.00002588838,0.99853885,0.0000013161817,0.0000067612946,0.00007816286,0.00003654013,0.00066920865,0.0005302008,0.000034037712,0.00007416335,0.00000166595],"about_ca_topic_score_codex":0.0014399765,"about_ca_topic_score_gemma":0.0014427031,"teacher_disagreement_score":0.0014399765,"about_ca_system_score_codex":0.00024261215,"about_ca_system_score_gemma":0.000060916012,"threshold_uncertainty_score":0.0031440854},"labels":[],"label_agreement":null},{"id":"W3203407363","doi":"10.3847/1538-4357/ac5027","title":"On the Accuracy of Underground Muon Intensity Calculations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Japan Society for the Promotion of Science","keywords":"Muon; Physics; Cosmic ray; Nuclear physics; Detector; Hadron; COSMIC cancer database; Lepton; Muon collider; Neutrino; Flux (metallurgy); Phase space; Particle physics; Particle accelerator; Astronomy; Beam (structure); Optics","score_opus":0.015778976464599206,"score_gpt":0.23727624793913965,"score_spread":0.22149727147454046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3203407363","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.40482268,0.0012443737,0.54098934,0.0009981446,0.00044788694,0.00006569679,0.0021658347,0.006594084,0.042671822],"genre_scores_gemma":[0.947791,0.00021803877,0.048117287,0.000121801626,0.000046642617,0.000047163452,0.0007206734,0.0010471047,0.001890249],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99868435,0.00045902902,0.0000745471,0.000191578,0.0004461294,0.00014442267],"domain_scores_gemma":[0.9919403,0.0045103068,0.0005099403,0.0017535537,0.0011093168,0.00017670989],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018393716,0.00079678115,0.00068811345,0.0011118598,0.0006758261,0.0014635483,0.002009113,0.0008073693,0.0045211595],"category_scores_gemma":[0.011874043,0.0003906381,0.0007014845,0.0009402891,0.0007416589,0.001694717,0.0016017214,0.001018713,0.0009239035],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017910181,0.000079071855,0.012040427,0.00014592875,0.00010851901,0.00020322298,0.00012263906,0.9178903,0.0040496374,0.036357015,0.002284453,0.026539644],"study_design_scores_gemma":[0.000013400323,0.000015802274,0.001132556,0.00004049365,0.00001295743,0.000026993139,0.0000306326,0.98769414,0.003975636,0.005868766,0.0011739664,0.0000146620105],"about_ca_topic_score_codex":0.012794782,"about_ca_topic_score_gemma":0.0059980894,"teacher_disagreement_score":0.012794782,"about_ca_system_score_codex":0.0009143723,"about_ca_system_score_gemma":0.0012065857,"threshold_uncertainty_score":0.025440633},"labels":[],"label_agreement":null},{"id":"W3203422577","doi":"10.3847/1538-4357/ac439a","title":"Dissecting Nearby Galaxies with piXedfit. I. Spatially Resolved Properties of Stars, Dust, and Gas as Revealed by Panchromatic SED Fitting","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; East Asian Core Observatories Association; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Vanderbilt University; Ulsan National Institute of Science and Technology; University of Oxford; Ministry of Science and Technology, Taiwan; York University; Carnegie Institution for Science; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; Academia Sinica; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Dust lane; Spectral energy distribution; Star formation; Spiral galaxy; Metallicity; Stars; Stellar mass; Astronomy; Stellar population; Circumstellar dust; Cosmic dust","score_opus":0.007024470783525915,"score_gpt":0.18962433727245256,"score_spread":0.18259986648892665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3203422577","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9746909,0.00014047812,0.018978076,0.000036491063,0.0000073797223,0.000018299963,0.0020815732,0.0030623067,0.0009845389],"genre_scores_gemma":[0.9607795,0.000057466856,0.0355355,0.000016122025,0.000008272422,0.000021664247,0.0028920989,0.00035027356,0.00033909566],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985576,0.000022740182,0.000011552411,0.000069441034,0.000027223627,0.000013362477],"domain_scores_gemma":[0.9995105,0.0001439973,0.00009487083,0.00013776401,0.00006676843,0.00004618457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050347735,0.000345818,0.00027423416,0.0014470967,0.00025262663,0.0005980047,0.00037454916,0.00018400744,0.0012840036],"category_scores_gemma":[0.0011243108,0.00023050935,0.0005194056,0.0012316979,0.00012853584,0.00030433811,0.0004273486,0.00016402491,0.00036442812],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039642333,0.00016011881,0.77269596,0.00013024012,0.00048744303,0.0006182038,0.0015825797,0.060472686,0.041764818,0.0014724097,0.0032591035,0.11696004],"study_design_scores_gemma":[0.000039570474,0.00010122276,0.6921139,0.000015785083,0.00011133378,0.00035794743,0.00040479816,0.2854163,0.01433297,0.00096375117,0.006108069,0.000034407236],"about_ca_topic_score_codex":0.0028476717,"about_ca_topic_score_gemma":0.003148919,"teacher_disagreement_score":0.0028476717,"about_ca_system_score_codex":0.000257647,"about_ca_system_score_gemma":0.00013228306,"threshold_uncertainty_score":0.005662203},"labels":[],"label_agreement":null},{"id":"W3203824826","doi":"10.3847/1538-4357/ac3490","title":"Low-J CO Line Ratios from Single-dish CO Mapping Surveys and PHANGS-ALMA","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Ministerio de Ciencia e Innovación; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; National Science Council; Deutsche Forschungsgemeinschaft; European Commission; Centre National d’Etudes Spatiales; Associated Universities; Agencia Estatal de Investigación; National Radio Astronomy Observatory; National Science Foundation; Compute Canada; Ministerio de Ciencia, Innovación y Universidades; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; Galaxy; Star formation; Line (geometry); Spiral galaxy; RADIUS; Astronomy; Geometry","score_opus":0.014647211130483928,"score_gpt":0.21955379553433818,"score_spread":0.20490658440385426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3203824826","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9850124,0.00012668982,0.002571707,0.00004555956,0.000013646376,0.000020995254,0.0032946598,0.00038644293,0.008527941],"genre_scores_gemma":[0.99080276,0.000054873875,0.0038182945,0.000027269038,0.00002340591,0.000018584273,0.0034858694,0.00006862447,0.0017002426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967945,0.000032456253,0.000013235764,0.00011956153,0.00010862847,0.000046621266],"domain_scores_gemma":[0.9992211,0.00008632161,0.00019004697,0.00018819988,0.0001410348,0.00017334496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033135223,0.00024231923,0.00023651637,0.0016171725,0.00024186427,0.00067081256,0.00033699762,0.00019033326,0.0028966884],"category_scores_gemma":[0.0010794315,0.00018277919,0.0002522293,0.0009317203,0.00018114707,0.0005228369,0.0005151989,0.00021737812,0.0012723658],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002223173,0.00008121144,0.881458,0.0000891032,0.00015522455,0.00016523016,0.00036588652,0.0031119788,0.037421208,0.0006762121,0.006275762,0.06997788],"study_design_scores_gemma":[0.0000057350103,0.00002005309,0.98844403,0.000007797426,0.000023048326,0.00006346295,0.00009616878,0.0036929757,0.0046566674,0.00020896041,0.002770843,0.000010272187],"about_ca_topic_score_codex":0.0049039815,"about_ca_topic_score_gemma":0.012428367,"teacher_disagreement_score":0.0049039815,"about_ca_system_score_codex":0.0003564986,"about_ca_system_score_gemma":0.00013208252,"threshold_uncertainty_score":0.009750843},"labels":[],"label_agreement":null},{"id":"W3204674667","doi":"10.3847/1538-4357/ac2ba2","title":"A Unified Model for the Fan Region and the North Polar Spur: A Bundle of Filaments in the Local Galaxy","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; National Research Council Canada; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Polar; Sky; Context (archaeology); Galaxy; Astrophysics; Astronomy; Bundle; Geography","score_opus":0.01778508329333579,"score_gpt":0.23822388018047486,"score_spread":0.22043879688713908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204674667","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4712473,0.0020624192,0.36554644,0.007265166,0.00020275531,0.00024172835,0.0007773325,0.000806482,0.15185046],"genre_scores_gemma":[0.96925807,0.00042229553,0.018894885,0.00021586505,0.00013270603,0.0001648345,0.00019161806,0.00006498161,0.010654763],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998735,0.00003739198,0.0000041437784,0.000029926281,0.000021938258,0.000033030417],"domain_scores_gemma":[0.9997638,0.00005019749,0.00004035698,0.000025342888,0.000039532915,0.00008068861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033298245,0.00042034878,0.00051345484,0.00078833645,0.0010864246,0.0018188485,0.0016866359,0.0015337339,0.0061917105],"category_scores_gemma":[0.00057639007,0.00032495652,0.0009759268,0.00038478954,0.0015126755,0.0023677973,0.0009543957,0.0005287086,0.00095957913],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049176135,0.000047236736,0.0042528557,0.000054699034,0.00003768682,0.0007819759,0.00059972017,0.12674771,0.003032695,0.856404,0.0027747247,0.005217505],"study_design_scores_gemma":[0.00008125151,0.00008405214,0.0031630353,0.000048979233,0.00004332257,0.0004507527,0.00037364644,0.58911455,0.00023616997,0.39740133,0.008963365,0.000039499104],"about_ca_topic_score_codex":0.0071900836,"about_ca_topic_score_gemma":0.0055991057,"teacher_disagreement_score":0.0071900836,"about_ca_system_score_codex":0.0010617615,"about_ca_system_score_gemma":0.00063913234,"threshold_uncertainty_score":0.02071333},"labels":[],"label_agreement":null},{"id":"W3204688037","doi":"10.3847/1538-4357/ac29b7","title":"Observation of the Gamma-Ray Binary HESS J0632+057 with the H.E.S.S., MAGIC, and VERITAS Telescopes","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; McGill University","funders":"Japan Aerospace Exploration Agency; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Bundesministerium für Bildung, Wissenschaft und Forschung; Australian Research Council; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Commission on Research, Science and Technology; Ministerio de Ciencia e Innovación; Institute for Cosmic Ray Research, University of Tokyo; Centre National de la Recherche Scientifique; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Hrvatska Zaklada za Znanost; Max-Planck-Gesellschaft; Japan Society for the Promotion of Science; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University of Tokyo; National Research Foundation; Austrian Science Fund; Office of Science; Academy of Finland; Universiteit van Amsterdam; University of Namibia; EGI Federation; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Ministry of Education, Culture, Sports, Science and Technology; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; National Energy Research Scientific Computing Center; Knut och Alice Wallenbergs Stiftelse; Narodowym Centrum Nauki; Generalitat de Catalunya; European Regional Development Fund; Bundesministerium für Bildung und Forschung; National Research Centre; Soochow University; U.S. Department of Energy; Smithsonian Institution; Alexander von Humboldt-Stiftung; California Institute of Technology; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Centres de Recerca de Catalunya; National Science Foundation","keywords":"Physics; Astrophysics; Gamma ray; Flux (metallurgy); Cherenkov radiation; Light curve; Astronomy; MAGIC (telescope); Orbital period; Stars; Optics","score_opus":0.011356046606679345,"score_gpt":0.20949571858208657,"score_spread":0.19813967197540722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204688037","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986534,0.00008088197,0.0000479085,0.000017913953,0.0000043498535,0.0000048289244,0.0005735245,0.0000136680965,0.000603405],"genre_scores_gemma":[0.9968215,0.000052457504,0.00036819433,0.000024609186,0.000010730645,0.0000075338908,0.0024280336,0.0000059796557,0.000280992],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998042,0.000019817171,0.0000130493745,0.000042774198,0.00007826102,0.000041969597],"domain_scores_gemma":[0.999602,0.000027789194,0.00012367802,0.000045437722,0.00006657038,0.00013451639],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034637956,0.000274429,0.00034027864,0.001172632,0.00046821494,0.00046383045,0.00027530824,0.00033946018,0.00089432765],"category_scores_gemma":[0.00037827762,0.00020363831,0.00018994746,0.0010381815,0.00023888539,0.00024542658,0.0005864344,0.00025283266,0.00036090234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010275431,0.00024682508,0.8730417,0.00012385285,0.00021002619,0.0010543014,0.0004809492,0.0009174364,0.10329958,0.00032270208,0.002147217,0.017127762],"study_design_scores_gemma":[0.000035605437,0.00018708297,0.99496526,0.000007978968,0.000025071871,0.00026254417,0.000101760066,0.0007578978,0.0020719448,0.000033643748,0.0015412517,0.000009968242],"about_ca_topic_score_codex":0.010004216,"about_ca_topic_score_gemma":0.022864604,"teacher_disagreement_score":0.010004216,"about_ca_system_score_codex":0.00046210753,"about_ca_system_score_gemma":0.00042079258,"threshold_uncertainty_score":0.019891977},"labels":[],"label_agreement":null},{"id":"W3204751258","doi":"10.3847/1538-4357/ac4973","title":"The High Latitude Spectroscopic Survey on the Nancy Grace Roman Space Telescope","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":119,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Science Mission Directorate; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Physics; Grism; Redshift; Galaxy; Astrophysics; Redshift survey; Astronomy; Telescope; Flux (metallurgy); Cosmic microwave background; Dark energy; Spitzer Space Telescope; Cosmology; Optics","score_opus":0.008568541845177783,"score_gpt":0.21415404721459247,"score_spread":0.2055855053694147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204751258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97581255,0.00011385795,0.007766522,0.0005350982,0.000045003075,0.00007167439,0.0016397209,0.00034195272,0.013673537],"genre_scores_gemma":[0.98820484,0.00006581205,0.0073382948,0.00010273664,0.000016061904,0.000049389288,0.002545447,0.00005583942,0.0016216735],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99968743,0.00013714706,0.000008275389,0.000061035564,0.000057490593,0.000048759535],"domain_scores_gemma":[0.9997254,0.000034797646,0.00003581685,0.000092425435,0.000055771332,0.00005572338],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000690761,0.00022961549,0.00032927727,0.00023344682,0.00040265793,0.00047672557,0.0005957343,0.00032546374,0.0013747378],"category_scores_gemma":[0.0013926877,0.00024041926,0.0004606667,0.00043114627,0.00034300247,0.0003850284,0.0007092536,0.0003824124,0.00038349812],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033318167,0.00016597513,0.20596944,0.00004881727,0.00019063236,0.0005418823,0.00024399138,0.73354733,0.008880838,0.017219301,0.01236938,0.020489259],"study_design_scores_gemma":[0.0002070501,0.00018326784,0.19755407,0.000019346431,0.00003640973,0.00014634104,0.00011554546,0.7780347,0.0025306935,0.0033727875,0.01773607,0.0000637154],"about_ca_topic_score_codex":0.03198557,"about_ca_topic_score_gemma":0.020897524,"teacher_disagreement_score":0.03198557,"about_ca_system_score_codex":0.0009634078,"about_ca_system_score_gemma":0.0005744718,"threshold_uncertainty_score":0.06359881},"labels":[],"label_agreement":null},{"id":"W3204758396","doi":"10.3847/1538-4357/ac3f3a","title":"Final Moments. I. Precursor Emission, Envelope Inflation, and Enhanced Mass Loss Preceding the Luminous Type II Supernova 2020tlf","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Grand Équipement National De Calcul Intensif; Science and Technology Facilities Council; University of Toronto; Nuclear Safety and Security Commission; Heising-Simons Foundation; Canadian Institute for Advanced Research; Northwestern University; Canada Research Chairs; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Light curve; Luminosity; Emission spectrum; Radiative transfer; Neutron star; Spectral line; Galaxy; Astronomy","score_opus":0.013780310716587495,"score_gpt":0.23634280983891082,"score_spread":0.22256249912232332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204758396","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972779,0.000064966545,0.0008363007,0.000015226993,0.0000034677564,0.0000067220944,0.00021702965,0.000059339283,0.0015191225],"genre_scores_gemma":[0.99894565,0.000014088644,0.00021944976,0.000006386897,0.0000021908568,0.0000031246427,0.00043519915,0.000006855258,0.00036708676],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999628,0.0000019439838,0.000001956926,0.000009193372,0.000008884895,0.00001517077],"domain_scores_gemma":[0.999897,0.0000120994155,0.000027452776,0.000009796947,0.000012439188,0.000041243973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010719684,0.000286163,0.00015668028,0.00036002704,0.00022561285,0.00043145093,0.00018999982,0.00024536502,0.0013030773],"category_scores_gemma":[0.00030386815,0.0001362,0.0003034767,0.0001248125,0.00014495067,0.00018519255,0.00038299427,0.000250328,0.00028293388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019550452,0.00023032687,0.7280721,0.00011523216,0.00012247522,0.0076534166,0.0005590294,0.0133979,0.21592021,0.005548049,0.0015050565,0.02492117],"study_design_scores_gemma":[0.000025553994,0.0004941544,0.94648826,0.000017221415,0.000030357816,0.0022380843,0.00015970685,0.024424955,0.022307754,0.0010136697,0.0027733324,0.000027060656],"about_ca_topic_score_codex":0.0026890363,"about_ca_topic_score_gemma":0.0023664269,"teacher_disagreement_score":0.0026890363,"about_ca_system_score_codex":0.00030826812,"about_ca_system_score_gemma":0.000094873,"threshold_uncertainty_score":0.0053468347},"labels":[],"label_agreement":null},{"id":"W3204836845","doi":"10.3847/1538-4357/ac5960","title":"Evolution of Primordial Magnetic Fields during Large-scale Structure Formation","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Laurentian University","funders":"Shota Rustaveli National Science Foundation; National Science Foundation; Vetenskapsrådet; National Research Foundation; European Commission; Volkswagen Foundation","keywords":"Physics; Universe; Magnetic field; Cosmology; Inflation (cosmology); Astrophysics; Theoretical physics; Quantum mechanics","score_opus":0.003102756117459319,"score_gpt":0.18314095836910282,"score_spread":0.1800382022516435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3204836845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977036,0.000027603106,0.0012309904,0.000042034753,0.0000036426563,0.000004542144,0.00009823123,0.00002486466,0.00086441543],"genre_scores_gemma":[0.9994592,0.000011851116,0.000363128,0.0000044423173,0.0000011993725,0.00000257491,0.00006668749,0.0000051451443,0.00008569248],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999442,0.00002227165,0.0000023388852,0.000009877586,0.00000775424,0.000013546858],"domain_scores_gemma":[0.9995646,0.00016612088,0.00008743818,0.00004509916,0.00003990077,0.00009674427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032055518,0.0001494788,0.0001732553,0.00024316259,0.00025985547,0.0005416782,0.00032548018,0.00033856524,0.0010056985],"category_scores_gemma":[0.0012656569,0.00011878264,0.00024689155,0.0002298834,0.00042992592,0.00031867207,0.00030481463,0.00032418047,0.0000864853],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035538175,0.00016985905,0.15001418,0.0000619782,0.00016813906,0.00033480884,0.00018040373,0.80423594,0.024694508,0.0139526725,0.00071421795,0.0051179244],"study_design_scores_gemma":[0.000096355645,0.00012802161,0.074288025,0.0000110032315,0.000035600904,0.000079081954,0.0000789205,0.9166254,0.0029984857,0.0050982395,0.00053915865,0.000021736902],"about_ca_topic_score_codex":0.0044194167,"about_ca_topic_score_gemma":0.0036990177,"teacher_disagreement_score":0.0044194167,"about_ca_system_score_codex":0.0006217791,"about_ca_system_score_gemma":0.00024399912,"threshold_uncertainty_score":0.008787394},"labels":[],"label_agreement":null},{"id":"W3205077328","doi":"10.3847/1538-4357/ac15f4","title":"Energy Transfer Across the Magnetopause Under Radial IMF Conditions","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"National Key Research and Development Program of China","keywords":"Magnetopause; Physics; Magnetosphere; Solar wind; Geophysics; Interplanetary magnetic field; Northern Hemisphere; Southern Hemisphere; Astrophysics; Atmospheric sciences; Magnetic field; Astronomy","score_opus":0.006346610787712425,"score_gpt":0.23072946335220784,"score_spread":0.22438285256449542,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3205077328","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925237,0.000119932025,0.003341457,0.000057758218,0.0000056270355,0.000007149611,0.0001490901,0.00009286677,0.0037023684],"genre_scores_gemma":[0.99929714,0.00004091793,0.00021299007,0.000004701312,0.0000019049074,0.0000026542784,0.000056634894,0.000008513983,0.00037448163],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99995375,0.000009267707,0.0000023415591,0.000008936397,0.000007967776,0.000017673052],"domain_scores_gemma":[0.9999269,0.000020397327,0.000017832754,0.000009953878,0.000012535176,0.000012303807],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012887114,0.00036983495,0.00025800665,0.0002598748,0.0002757706,0.00034956905,0.00031218128,0.00029640607,0.0019319574],"category_scores_gemma":[0.0005559776,0.00015708117,0.0004028816,0.00018860098,0.00019356131,0.0005612984,0.000525538,0.00020432427,0.00020892035],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065054186,0.00008321298,0.099721596,0.00012376158,0.00012243619,0.0010538371,0.0002706813,0.8117212,0.06396945,0.0046722307,0.0006616048,0.016949428],"study_design_scores_gemma":[0.00005681027,0.0001706275,0.04503698,0.000012818341,0.000048331643,0.00020628807,0.00019181315,0.943939,0.0082182875,0.0014121148,0.000682635,0.000024346984],"about_ca_topic_score_codex":0.0044714184,"about_ca_topic_score_gemma":0.0012818439,"teacher_disagreement_score":0.0044714184,"about_ca_system_score_codex":0.0002919821,"about_ca_system_score_gemma":0.00017612251,"threshold_uncertainty_score":0.008890808},"labels":[],"label_agreement":null},{"id":"W3205120522","doi":"10.3847/1538-4357/ac2eb4","title":"Mapping Obscuration to Reionization with ALMA (MORA): 2 mm Efficiently Selects the Highest-redshift Obscured Galaxies","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Institutes of Natural Sciences; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Astronomical Observatory of Japan; Danmarks Grundforskningsfond; National Research Foundation; Ministero dell’Istruzione, dell’Università e della Ricerca; Natural Sciences and Engineering Research Council of Canada; Flatiron Health; Comisión Nacional de Investigación Científica y Tecnológica; Associated Universities; University of Texas at Austin; National Radio Astronomy Observatory; Max-Planck-Gesellschaft; Simons Foundation; Villum Fonden; Research Corporation for Science Advancement; National Science Foundation","keywords":"Physics; Reionization; Galaxy; Redshift; Astrophysics; Astronomy; Intergalactic medium","score_opus":0.0074852560034922005,"score_gpt":0.20219947779541197,"score_spread":0.19471422179191977,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3205120522","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928732,0.00012765288,0.0022538132,0.00005660031,0.000004522283,0.000014270447,0.0014097367,0.00047487995,0.0027853318],"genre_scores_gemma":[0.9948211,0.00002825937,0.0026108676,0.00003308919,0.000011731142,0.000012765879,0.001716265,0.00006136821,0.0007045701],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975055,0.00004726307,0.000011546788,0.0000691567,0.00006085488,0.000060507602],"domain_scores_gemma":[0.99886155,0.00017289615,0.00034321076,0.00027409956,0.00015644405,0.00019182335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046838835,0.00033915965,0.0003057967,0.001343188,0.00023388391,0.0008160492,0.00037489316,0.00019254704,0.0027224608],"category_scores_gemma":[0.0010137231,0.0002137377,0.0003230285,0.00069377007,0.00013614522,0.00035153178,0.0006040207,0.00019492499,0.0008635951],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026212286,0.000055704586,0.93155,0.000037895752,0.000093344046,0.000143156,0.00031207013,0.0007776954,0.037266996,0.00025858326,0.0020068067,0.02723564],"study_design_scores_gemma":[0.0000087033195,0.000033022156,0.9933351,0.000005117433,0.000020085128,0.00008950776,0.00006309217,0.0015524812,0.0032820564,0.00010145053,0.0015016013,0.0000076165657],"about_ca_topic_score_codex":0.0033029404,"about_ca_topic_score_gemma":0.00745999,"teacher_disagreement_score":0.0033029404,"about_ca_system_score_codex":0.00026127175,"about_ca_system_score_gemma":0.00015010295,"threshold_uncertainty_score":0.00910759},"labels":[],"label_agreement":null},{"id":"W3205653761","doi":"10.3847/1538-4357/ac399b","title":"From the Fire: A Deeper Look at the Phoenix Stream","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"SLAC National Accelerator Laboratory; Integrated Electronics Engineering Center, Binghamton University; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Office of Science; Institut de Física d'Altes Energies; ARC Centre of Excellence for All-Sky Astrophysics; Generalitat de Catalunya; European Regional Development Fund; U.S. Department of Energy; European Commission; Science and Technology Facilities Council; University College London; Argonne National Laboratory; Centres de Recerca de Catalunya; High Energy Physics; Deutsche Forschungsgemeinschaft; University of Portsmouth; Ohio State University; University of Illinois at Urbana-Champaign; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; University of Sussex; Ministério da Ciência, Tecnologia e Inovação; University of Chicago; Fermilab; National Science Foundation","keywords":"Phoenix; Physics; Astrophysics; Metallicity; Degree (music); Baryon; Galaxy; Geography","score_opus":0.012537931775061581,"score_gpt":0.23180421771109017,"score_spread":0.2192662859360286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3205653761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957281,0.00010383794,0.0009058276,0.00016127768,0.0000063137945,0.000007055433,0.0011584966,0.00003310035,0.0018959801],"genre_scores_gemma":[0.99540883,0.00015493776,0.0012095087,0.00004808893,0.0000169779,0.0000036378703,0.0019829196,0.00003426367,0.0011408612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990237,0.000010716111,0.000004377659,0.000044350676,0.000019969379,0.000018157061],"domain_scores_gemma":[0.99967504,0.00006862826,0.00009099314,0.00004497044,0.000054472075,0.000065901666],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000352274,0.00019507579,0.00026165167,0.000964998,0.000370325,0.0013150552,0.00029354967,0.00035853506,0.0023269088],"category_scores_gemma":[0.001195803,0.000120948775,0.00021815594,0.0012051705,0.00028256347,0.00083179603,0.0006714371,0.0005111802,0.00026938],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022545116,0.00006690815,0.96172786,0.000034780147,0.000130833,0.00073051325,0.0007601742,0.007743287,0.0068321726,0.0016302684,0.0015429883,0.018574622],"study_design_scores_gemma":[0.000013026506,0.000032959593,0.96830887,0.00002250903,0.000029612684,0.00016178504,0.00058158365,0.02144635,0.0018838423,0.00070429465,0.006801792,0.000013443295],"about_ca_topic_score_codex":0.021250919,"about_ca_topic_score_gemma":0.019208876,"teacher_disagreement_score":0.021250919,"about_ca_system_score_codex":0.0005963669,"about_ca_system_score_gemma":0.00021766766,"threshold_uncertainty_score":0.042254448},"labels":[],"label_agreement":null},{"id":"W3205830330","doi":"10.3847/1538-4357/ac2302","title":"Rotation Curves of Galaxies and Their Dependence on Morphology and Stellar Mass","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Galaxy rotation curve; Galaxy; Astronomy; Rotation (mathematics); Stellar mass; Stellar rotation; Stars; Galaxy formation and evolution; Star formation; Geometry","score_opus":0.011516783938735653,"score_gpt":0.22218891370445928,"score_spread":0.21067212976572364,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3205830330","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969195,0.0001584687,0.0008180938,0.000028052278,0.0000029849919,0.000003133957,0.0011778366,0.00009482545,0.00079707656],"genre_scores_gemma":[0.998256,0.00003526996,0.00021092404,0.0000025781558,0.000003671728,0.0000016916119,0.0013624685,0.000018465276,0.00010891995],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995065,0.0001377586,0.000034947716,0.00015458703,0.00008141753,0.00008489692],"domain_scores_gemma":[0.99365366,0.0026044736,0.0017688558,0.0007344997,0.0007518971,0.00048654864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00075082935,0.00025402097,0.00023423762,0.0023193704,0.00018577176,0.0007503372,0.00018430664,0.00024589992,0.0013061727],"category_scores_gemma":[0.008539699,0.00014248402,0.00032421818,0.0018295681,0.00035423943,0.00053976226,0.00039837844,0.00022131317,0.0006579295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041919513,0.0000050580425,0.9928404,0.000005517833,0.00004090485,0.000026862308,0.00005822097,0.0012247139,0.000944797,0.000073153635,0.00015131182,0.0045872424],"study_design_scores_gemma":[8.665504e-7,0.000017369808,0.99623674,0.000002298769,0.0000059608647,0.000063301755,0.000046518875,0.0030452963,0.00023159129,0.00006333835,0.00028165377,0.00000491736],"about_ca_topic_score_codex":0.006089828,"about_ca_topic_score_gemma":0.004027205,"teacher_disagreement_score":0.006089828,"about_ca_system_score_codex":0.00023910253,"about_ca_system_score_gemma":0.00011904743,"threshold_uncertainty_score":0.012108803},"labels":[],"label_agreement":null},{"id":"W3206532571","doi":"10.3847/1538-4357/ac2df1","title":"The Far-away Blues: Exploring the Furthest Extents of the Boötes I Ultra-faint Dwarf Galaxy","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; National Astronomical Observatories, Chinese Academy of Sciences; Office of Science; Max-Planck-Institut für Astronomie; Smithsonian Astrophysical Observatory; National Development and Reform Commission; National Central University; Chinese Academy of Sciences; Queen's University Belfast; Durham University; York University; Space Telescope Science Institute; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Harvard University; Queen's University; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University","keywords":"Physics; Astrophysics; Astronomy; Stars; Astrometry; Galaxy; Milky Way; Dwarf galaxy; Stellar population; Red-giant branch; Photometry (optics); Population; Horizontal branch; Satellite galaxy; Blue straggler; Star cluster; Star formation; Globular cluster","score_opus":0.02064511457603675,"score_gpt":0.2236766431302465,"score_spread":0.20303152855420975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3206532571","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986871,0.00006395559,0.00021795984,0.000010900268,5.820902e-7,8.865384e-7,0.00003880775,0.0000049598084,0.0009747832],"genre_scores_gemma":[0.999546,0.00002539453,0.00015913065,0.000006116913,0.0000013360483,6.1647387e-7,0.000069606605,0.000002294501,0.00018942918],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999409,0.0000066210737,0.000002723567,0.000020171856,0.000012730314,0.000016837734],"domain_scores_gemma":[0.9997471,0.000046921898,0.0000710848,0.000028660443,0.000029214878,0.00007710268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014792729,0.00010473815,0.00016120097,0.00081737764,0.0003133436,0.0005163648,0.00017178402,0.000117743686,0.0010806235],"category_scores_gemma":[0.0003531587,0.00008371257,0.000117159965,0.0002724615,0.0003112757,0.00037934858,0.0008105514,0.0001396217,0.00016928901],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008524564,0.000018068518,0.9548745,0.000021729626,0.00003072632,0.000103276565,0.001346751,0.00038798322,0.02860983,0.0008257931,0.00010506934,0.013591117],"study_design_scores_gemma":[0.0000014074407,0.000028035887,0.99716216,0.0000058351147,0.0000052968035,0.000056795554,0.00070489343,0.00039361452,0.0007848011,0.00023807562,0.0006167672,0.0000021310555],"about_ca_topic_score_codex":0.004097105,"about_ca_topic_score_gemma":0.010640416,"teacher_disagreement_score":0.004097105,"about_ca_system_score_codex":0.00020265896,"about_ca_system_score_gemma":0.00009934523,"threshold_uncertainty_score":0.008146524},"labels":[],"label_agreement":null},{"id":"W3206680518","doi":"10.3847/1538-4357/ac46d3","title":"S <sup>5</sup>: The Orbital and Chemical Properties of One Dozen Stellar Streams","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":91,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; University of Illinois at Urbana-Champaign; Institut de Física d'Altes Energies; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University of New South Wales; Deutsche Forschungsgemeinschaft; University of Edinburgh; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; University of Sussex; University of Nottingham; National Aeronautics and Space Administration; University College London; SLAC National Accelerator Laboratory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Australian Research Council; Space Telescope Science Institute; University of Portsmouth; University of Chicago; Ohio State University; Ministério da Ciência, Tecnologia e Inovação; Fermilab; National Science Foundation; European Space Agency; University of Michigan; U.S. Department of Energy; University of Cambridge","keywords":"Physics; Metallicity; STREAMS; Astrophysics; Milky Way; Galaxy; Globular cluster; Astronomy","score_opus":0.015419829981750037,"score_gpt":0.22517072920372463,"score_spread":0.2097508992219746,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3206680518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970509,0.00008547768,0.00021405493,0.000009138511,0.0000030159474,0.000005640284,0.0016877791,0.000027728265,0.00091621646],"genre_scores_gemma":[0.98972636,0.00006510869,0.0007623904,0.000012597892,0.000017008542,0.00000737654,0.008655104,0.000019275649,0.00073470635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998617,0.00000928281,0.000018615629,0.00004075585,0.000039586663,0.000030109599],"domain_scores_gemma":[0.99919564,0.00009164744,0.00028863444,0.000084339124,0.00018924038,0.0001504873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029942903,0.00019328835,0.00021625665,0.0015186643,0.000401845,0.00074593624,0.00019343272,0.000171785,0.0023249693],"category_scores_gemma":[0.00078899635,0.0000785238,0.00020541878,0.0011536606,0.00019137327,0.00035599832,0.00041385822,0.00011427375,0.001220647],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017292486,0.000034886056,0.97887796,0.000015835467,0.000025400073,0.000099551675,0.00015115952,0.00027562227,0.0061637657,0.000121052115,0.000486711,0.013575191],"study_design_scores_gemma":[0.0000053512226,0.00009154007,0.9915558,0.0000067242504,0.000028138638,0.00031230974,0.00021165272,0.001295946,0.0034360853,0.00012727165,0.0029238537,0.0000052142814],"about_ca_topic_score_codex":0.0020561705,"about_ca_topic_score_gemma":0.0033987823,"teacher_disagreement_score":0.0023249693,"about_ca_system_score_codex":0.00021465184,"about_ca_system_score_gemma":0.00014540972,"threshold_uncertainty_score":0.00777781},"labels":[],"label_agreement":null},{"id":"W3206737128","doi":"10.3847/1538-4357/ac562a","title":"Minkowski Functionals of SDSS-III BOSS: Hints of Possible Anisotropy in the Density Field?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Brookhaven National Laboratory; York University; National Energy Research Scientific Computing Center; Ohio State University; National Research Foundation; Carnegie Mellon University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; National Science Foundation; Lawrence Berkeley National Laboratory; Ministry of Science and ICT, South Korea; National Research Foundation of Korea; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; University of Arizona; Barcelona Supercomputing Center; European Commission; U.S. Department of Energy","keywords":"Minkowski space; Physics; Galaxy; Smoothing; Amplitude; Gaussian; Cosmology; Gaussian random field; Astrophysics; Statistical physics; Gaussian process; Mathematical physics; Mathematics; Statistics; Quantum mechanics","score_opus":0.008486902250805539,"score_gpt":0.21845870595627237,"score_spread":0.20997180370546684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3206737128","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9877066,0.00007444075,0.0066061043,0.000077756835,0.0000056216095,0.0000064112755,0.0018035833,0.00025936202,0.0034599632],"genre_scores_gemma":[0.9970983,0.00001860801,0.0012073066,0.000009348446,0.0000055805726,0.000004621465,0.0014759382,0.000040185452,0.00014012503],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99956065,0.00013091121,0.000030262265,0.00007982433,0.00012185567,0.00007644821],"domain_scores_gemma":[0.9981153,0.0004889503,0.0005046371,0.00046580983,0.00021830235,0.00020703646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012933508,0.0002861196,0.00030713517,0.002004058,0.00027171025,0.00079507544,0.00022069199,0.00014775038,0.001373023],"category_scores_gemma":[0.0033397677,0.00017830718,0.00026042073,0.0013761413,0.0006174389,0.00054985506,0.0004727447,0.00024135887,0.00039794328],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062195346,0.000066426684,0.8191213,0.00020085082,0.00021524524,0.00022289433,0.00095857616,0.020327035,0.065328255,0.043607146,0.00443096,0.044899464],"study_design_scores_gemma":[0.000008625838,0.000024535655,0.9565045,0.000017720196,0.000012032973,0.00014602234,0.0001620815,0.026672946,0.0081490185,0.005324581,0.002938398,0.00003948129],"about_ca_topic_score_codex":0.0025539594,"about_ca_topic_score_gemma":0.0022608808,"teacher_disagreement_score":0.0025539594,"about_ca_system_score_codex":0.00044659947,"about_ca_system_score_gemma":0.00017992366,"threshold_uncertainty_score":0.006839931},"labels":[],"label_agreement":null},{"id":"W3207037174","doi":"10.3847/1538-4357/ac31b0","title":"Galactic Chemical Evolution of Radioactive Isotopes with an s-process Contribution","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"European Research Council; European Cooperation in Science and Technology; Science and Technology Facilities Council; National Science Foundation","keywords":"Nucleosynthesis; Physics; Metallicity; Astrophysics; Stars; Asymptotic giant branch; s-process; Presolar grains; Meteorite; Supernova; Isotope; Astronomy; Nuclear physics","score_opus":0.0042490915885948595,"score_gpt":0.20782669023210623,"score_spread":0.20357759864351138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207037174","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99753225,0.00005001547,0.0010153007,0.000021829106,0.0000023886569,0.000003822855,0.00015766769,0.000035245765,0.0011814728],"genre_scores_gemma":[0.99919766,0.000021192556,0.00031631053,0.0000046277873,0.000001050109,0.0000026830387,0.00019058282,0.000015156329,0.00025067054],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999223,0.0000126070145,0.0000054851876,0.000031291398,0.000014338412,0.000014066059],"domain_scores_gemma":[0.999559,0.00016345111,0.00008996839,0.00004054791,0.0001027981,0.00004416091],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030416495,0.00040270493,0.00019444774,0.0005758843,0.00030801664,0.0007608461,0.00051923457,0.00047747753,0.00090183853],"category_scores_gemma":[0.0010995142,0.00029395657,0.0004285907,0.0003838174,0.00032316064,0.00039592356,0.00028398866,0.00023991597,0.00023385293],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004978872,0.00010566776,0.48261282,0.000064381355,0.00019588345,0.00058988365,0.00012324065,0.44689327,0.054825418,0.005880512,0.00031424116,0.007896844],"study_design_scores_gemma":[0.000071858274,0.00020800022,0.1296224,0.000013605849,0.00009579298,0.00025429853,0.00009617094,0.83461916,0.03192254,0.0016981057,0.0013565685,0.00004137574],"about_ca_topic_score_codex":0.007145271,"about_ca_topic_score_gemma":0.0036573277,"teacher_disagreement_score":0.007145271,"about_ca_system_score_codex":0.0011236913,"about_ca_system_score_gemma":0.00021313534,"threshold_uncertainty_score":0.014207363},"labels":[],"label_agreement":null},{"id":"W3207059346","doi":"10.3847/1538-4357/acbb5f","title":"Weighing the Darkness. II. Astrometric Measurement of Partial Orbits with Gaia","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Seventh Framework Programme; University of Crete; Danmarks Grundforskningsfond; National Research Foundation; Department of Atomic Energy, Government of India; European Commission; Aspen Center for Physics; Northwestern University; National Science Foundation","keywords":"Physics; Astrometry; Astronomy; Astrophysics; Stars; Exoplanet; Orbit (dynamics); Parallax; Proper motion; Orbital elements; Population; Orbital motion; Angular momentum; Classical mechanics","score_opus":0.022948357797376726,"score_gpt":0.22559512243106575,"score_spread":0.20264676463368902,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207059346","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99068797,0.00016079514,0.0045207986,0.000055368826,0.000019526859,0.000013410557,0.0007383834,0.00019646545,0.003607333],"genre_scores_gemma":[0.9968286,0.000024732506,0.002629146,0.000015286654,0.0000048953393,0.0000035334062,0.00026847995,0.000015951597,0.00020935418],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976796,0.000062600455,0.000013374767,0.00006981128,0.00005725818,0.000029095732],"domain_scores_gemma":[0.9989944,0.000140043,0.00033926516,0.00022638329,0.0001827317,0.0001172516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044341732,0.00023620267,0.00016022038,0.001584848,0.00040488038,0.0005351566,0.00027426894,0.00024401191,0.00072363],"category_scores_gemma":[0.0024694002,0.00015131352,0.00015485844,0.00095454836,0.0003908469,0.0005599425,0.0006723576,0.00029207038,0.0002985075],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028950203,0.00003722077,0.9158114,0.000048664442,0.00011083241,0.000101533995,0.00047977897,0.0035316579,0.04006247,0.0019051002,0.00080363406,0.036818236],"study_design_scores_gemma":[0.000005006971,0.00010103597,0.9711052,0.000013305172,0.000027516424,0.00030031128,0.0002050437,0.013581142,0.011752698,0.0009082946,0.0019800975,0.00002040814],"about_ca_topic_score_codex":0.0021094629,"about_ca_topic_score_gemma":0.004337902,"teacher_disagreement_score":0.0021094629,"about_ca_system_score_codex":0.0003397368,"about_ca_system_score_gemma":0.00012632621,"threshold_uncertainty_score":0.004194379},"labels":[],"label_agreement":null},{"id":"W3207091279","doi":"10.3847/1538-4357/ac300a","title":"Stellar Rotation of T Tauri Stars in the Orion Star-forming Complex","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"T Tauri star; Physics; Stars; Astrophysics; Algorithm; Computer science","score_opus":0.02042154613072149,"score_gpt":0.24587535281368816,"score_spread":0.22545380668296666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207091279","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984255,0.00014834119,0.0001959443,0.000015278689,0.0000015048005,0.000004829144,0.00040986703,0.000013418653,0.00078535266],"genre_scores_gemma":[0.9986809,0.00008738388,0.00022894172,0.0000071500326,0.000008452602,0.0000046829614,0.000747502,0.0000120576115,0.00022289604],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997434,0.00005267302,0.000018161587,0.000091155525,0.00004704194,0.000047620382],"domain_scores_gemma":[0.9992411,0.00015238581,0.00022852138,0.0000962272,0.000112416266,0.00016942812],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043622503,0.00035318176,0.00029016112,0.0016238698,0.00045476438,0.00073778426,0.00023469793,0.00018870675,0.0010092153],"category_scores_gemma":[0.0010552633,0.00008952161,0.00025949598,0.0015235447,0.0002717053,0.0004250754,0.0005870274,0.00018398359,0.0004144931],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010618024,0.00003500962,0.9869849,0.000020637208,0.00004614756,0.00014873476,0.00043394166,0.000732968,0.004678293,0.00012799053,0.00022657531,0.006458489],"study_design_scores_gemma":[0.0000033881252,0.000035297566,0.9976987,0.000003154904,0.000014046871,0.00007728108,0.00013592413,0.0007756498,0.00046499062,0.000042846033,0.0007443544,0.000004350613],"about_ca_topic_score_codex":0.007519878,"about_ca_topic_score_gemma":0.00506165,"teacher_disagreement_score":0.007519878,"about_ca_system_score_codex":0.00047774112,"about_ca_system_score_gemma":0.00018272604,"threshold_uncertainty_score":0.014952183},"labels":[],"label_agreement":null},{"id":"W3207492739","doi":"10.3847/1538-4357/ac2f40","title":"Finite-resolution Deconvolution of Multiwavelength Imaging of 20,000 Galaxies in the COSMOS Field: The Evolution of Clumpy Galaxies over Cosmic Time","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Redshift; Stellar mass; Star formation; Surface brightness; Hubble Ultra-Deep Field; Deconvolution; COSMIC cancer database; Astronomy; Hubble Deep Field","score_opus":0.005608647427648816,"score_gpt":0.21086315976325476,"score_spread":0.20525451233560593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207492739","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99524766,0.00008319895,0.004200274,0.000020455524,0.0000026061027,0.000003118121,0.00013686663,0.000085573345,0.00022032572],"genre_scores_gemma":[0.9947296,0.000042296444,0.004775264,0.0000078907005,0.0000032132402,0.000002601402,0.00033415027,0.000019453924,0.000085618325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999069,0.000012896666,0.0000043936857,0.000030148774,0.000022513128,0.00002307743],"domain_scores_gemma":[0.99940395,0.00016042202,0.00015876911,0.00009884521,0.000094530005,0.000083477185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076909794,0.00020645103,0.00016213358,0.001025995,0.000183075,0.0003584127,0.00037436318,0.00022922657,0.0003668231],"category_scores_gemma":[0.0013086892,0.00015821504,0.00041728574,0.0005194764,0.00027100343,0.00033387952,0.00030782024,0.00018465264,0.000093610295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004958005,0.00021337836,0.6466046,0.00012787247,0.000310213,0.0003858797,0.00044747422,0.12371784,0.17373104,0.0015257618,0.0005995924,0.051840488],"study_design_scores_gemma":[0.0000105153185,0.000051015293,0.7823118,0.00001341379,0.000035778055,0.00021227928,0.000103092345,0.19841062,0.017839316,0.00048607757,0.00050461857,0.00002148128],"about_ca_topic_score_codex":0.005782357,"about_ca_topic_score_gemma":0.0059979754,"teacher_disagreement_score":0.005782357,"about_ca_system_score_codex":0.0004909037,"about_ca_system_score_gemma":0.00020769607,"threshold_uncertainty_score":0.011497438},"labels":[],"label_agreement":null},{"id":"W3207517111","doi":"10.3847/1538-4357/ac8356","title":"Quasars with Periodic Variability: Capabilities and Limitations of Bayesian Searches for Supermassive Black Hole Binaries in Time-domain Surveys","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Supermassive black hole; Quasar; Physics; Parameter space; Light curve; Astrophysics; Binary number; Amplitude; Galaxy; Bayesian probability; Black hole (networking); Time domain; Observatory; Algorithm; Computer science; Statistics; Mathematics; Artificial intelligence","score_opus":0.014941222393969469,"score_gpt":0.21558834370098245,"score_spread":0.20064712130701298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207517111","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9839991,0.0002473372,0.014216004,0.0003134448,0.0000054684456,0.000022016327,0.00011862525,0.0000808795,0.0009970193],"genre_scores_gemma":[0.9955023,0.00006274171,0.004213941,0.000026551063,0.0000052539153,0.000012413699,0.00007760908,0.000011498502,0.00008768877],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99898106,0.0006625142,0.000039053702,0.00011807253,0.00011290406,0.00008636641],"domain_scores_gemma":[0.986508,0.010948692,0.0011095679,0.0005892194,0.0004933005,0.00035112983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0056603164,0.00043843035,0.0005989113,0.00094729144,0.00057259755,0.001113244,0.00095776335,0.0009017345,0.0005674706],"category_scores_gemma":[0.020224415,0.0005164069,0.0005888035,0.00058011856,0.0007132952,0.0013870378,0.00080068456,0.0005763906,0.0000693356],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012657348,0.00006795283,0.061527662,0.000030668958,0.000094007795,0.00006248101,0.0001102101,0.92519826,0.00070714636,0.003924178,0.00022140777,0.007929493],"study_design_scores_gemma":[0.000019606963,0.000043189182,0.0050226822,0.000010220257,0.000013039872,0.000019373381,0.000027633643,0.99312556,0.00019827353,0.0014318821,0.000075811964,0.000012734378],"about_ca_topic_score_codex":0.023841457,"about_ca_topic_score_gemma":0.015989417,"teacher_disagreement_score":0.023841457,"about_ca_system_score_codex":0.0007744517,"about_ca_system_score_gemma":0.0006947685,"threshold_uncertainty_score":0.04740542},"labels":[],"label_agreement":null},{"id":"W3207606944","doi":"10.3847/1538-4357/ac54bd","title":"Quiescent Galaxy Size, Velocity Dispersion, and Dynamical Mass Evolution","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Astrophysics; Physics; Redshift; Velocity dispersion; Galaxy; Stellar mass; RADIUS; Galaxy formation and evolution; Population; Dark matter; Universe; Redshift survey; Astronomy; Star formation; Demography","score_opus":0.005964158139079136,"score_gpt":0.21229503693611723,"score_spread":0.2063308787970381,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207606944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864453,0.000020751291,0.00023933602,0.000005869414,4.7689406e-7,0.0000017922704,0.00057533017,0.000009409274,0.00050244527],"genre_scores_gemma":[0.9987936,0.000008257706,0.00014174735,0.0000026876914,0.0000014218627,0.0000012446493,0.0009172899,0.000002166176,0.00013145967],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998703,0.000028972167,0.000008251958,0.000038897404,0.000027577154,0.00002605212],"domain_scores_gemma":[0.99822456,0.0005238738,0.00062306615,0.00020491143,0.00017686922,0.00024670217],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045063655,0.00014025913,0.00015482004,0.0012086602,0.00017681357,0.00041109495,0.00019963621,0.0001318437,0.0012643256],"category_scores_gemma":[0.0019282417,0.00007869584,0.00018350701,0.0008190782,0.0003643738,0.00034287854,0.00034565153,0.00011613953,0.00018954692],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006510187,0.000021507274,0.9932088,0.0000061905157,0.000028541624,0.000026208558,0.00008601588,0.000751971,0.0028739485,0.00035575614,0.00012806409,0.0024478643],"study_design_scores_gemma":[0.0000018971236,0.000013871614,0.998288,0.0000010013495,0.0000041476524,0.000023879045,0.00002004239,0.0009178713,0.00048047543,0.0000860234,0.00016100021,0.0000018430038],"about_ca_topic_score_codex":0.005542314,"about_ca_topic_score_gemma":0.0068195197,"teacher_disagreement_score":0.005542314,"about_ca_system_score_codex":0.00023258103,"about_ca_system_score_gemma":0.000091734335,"threshold_uncertainty_score":0.011020124},"labels":[],"label_agreement":null},{"id":"W3207786568","doi":"10.3847/1538-4357/ac1343","title":"The Physics of the Coronal-line Region for Galaxies in Mapping Galaxies at Apache Point Observatory","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; University of Leicester; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Astronomy; Photoionization; Supernova; Observatory; Sky; Extragalactic astronomy; Line (geometry); Ionization","score_opus":0.024340565749808925,"score_gpt":0.22512082868213162,"score_spread":0.2007802629323227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207786568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982747,0.00008984663,0.0003099592,0.000045146455,0.0000017270692,0.0000046018426,0.00032124604,0.00002810842,0.00092470564],"genre_scores_gemma":[0.9991948,0.000025378758,0.0002655559,0.000012053546,0.0000033373606,0.000002176956,0.00029642732,0.000004339401,0.0001959934],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998727,0.00001360726,0.000005220986,0.000043897933,0.000032530148,0.000032031865],"domain_scores_gemma":[0.99916315,0.00011833802,0.00036418537,0.00006252924,0.000093229086,0.00019850385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002712601,0.00010934977,0.00010042343,0.0011085221,0.00037491941,0.0009036117,0.00030419743,0.00017894075,0.0017431654],"category_scores_gemma":[0.0007655002,0.00010447661,0.00014156921,0.0007010124,0.00027237163,0.0004909926,0.00055463874,0.00016729489,0.00016959841],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00001141124,0.0000123654445,0.99400055,0.0000059549025,0.000008377458,0.00005908553,0.0001548074,0.00021183025,0.0020705932,0.00026309883,0.00030063282,0.0029014007],"study_design_scores_gemma":[0.0000012348539,0.0000063251928,0.9983393,0.000003259652,0.0000024335259,0.00004842172,0.00014228447,0.0008421153,0.00022919607,0.00011252795,0.00027129494,0.0000014039806],"about_ca_topic_score_codex":0.01004256,"about_ca_topic_score_gemma":0.013850199,"teacher_disagreement_score":0.01004256,"about_ca_system_score_codex":0.0005769418,"about_ca_system_score_gemma":0.00013808953,"threshold_uncertainty_score":0.019968212},"labels":[],"label_agreement":null},{"id":"W3207969326","doi":"10.3847/1538-4357/ac1117","title":"The GOGREEN Survey: Evidence of an Excess of Quiescent Disks in Clusters at 1.0 &lt; z &lt; 1.4","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; York University; University of Waterloo","funders":"Astrophysics Division; Institut national des sciences de l'Univers; Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Ministerio de Ciencia, Tecnología e Innovación Productiva; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; California Institute of Technology; Academia Sinica; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Population; Galaxy cluster; Cluster (spacecraft); Mass ratio; Star formation; Accretion (finance); Oblate spheroid; Field galaxy; Redshift; Redshift survey; Atomic physics","score_opus":0.01954762155630298,"score_gpt":0.2597154650586496,"score_spread":0.24016784350234663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3207969326","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808335,0.0000765673,0.000055399378,0.000048476893,0.0000011209663,0.0000027232845,0.0009348904,0.000030793257,0.0007666774],"genre_scores_gemma":[0.9975061,0.0000622555,0.00011062295,0.00004697679,0.000006100466,0.0000046844166,0.0016634496,0.000015248251,0.0005846487],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980325,0.000013135591,0.000007389848,0.00005625491,0.00005193102,0.00006799798],"domain_scores_gemma":[0.99879456,0.000075453514,0.0004840125,0.00008293573,0.00016500991,0.00039804407],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000250758,0.00018701423,0.00026006319,0.002204941,0.0003821347,0.00062154623,0.00037431394,0.00020965848,0.0026649565],"category_scores_gemma":[0.0006542731,0.00015528029,0.000120599485,0.001144939,0.00034606038,0.00037699263,0.00083405763,0.0001713706,0.0006639178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005027415,0.000008943138,0.99348044,0.0000079615,0.000012340731,0.000049821723,0.00024374867,0.00002302836,0.0034876883,0.00007227743,0.00056817377,0.0019953565],"study_design_scores_gemma":[7.6959e-7,0.0000026134899,0.99965286,7.789862e-7,0.0000018419157,0.000015576159,0.00004798527,0.000015294567,0.000054167922,0.0000068559784,0.00020042047,7.7154476e-7],"about_ca_topic_score_codex":0.01751914,"about_ca_topic_score_gemma":0.038003415,"teacher_disagreement_score":0.01751914,"about_ca_system_score_codex":0.0003742886,"about_ca_system_score_gemma":0.00015588988,"threshold_uncertainty_score":0.034834325},"labels":[],"label_agreement":null},{"id":"W3208024764","doi":"10.3847/1538-4357/ac1418","title":"Ultracool Dwarfs Observed with the Spitzer Infrared Spectrograph. I. An Accurate Look at the L-to-T Transition at ∼300 Myr from Optical Through Mid-infrared Spectrophotometry","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Los Alamos National Laboratory; National Nuclear Security Administration; U.S. Department of Energy","keywords":"Astrophysics; Physics; Brown dwarf; Photometry (optics); Surface gravity; Infrared; Astronomy; Spectral energy distribution; Stars; Spectral line; Parallax; Galaxy","score_opus":0.016160536190166736,"score_gpt":0.23252571234971559,"score_spread":0.21636517615954884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208024764","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99866235,0.000061938896,0.0002678274,0.000009785727,0.0000013103712,0.0000024252531,0.00040806955,0.000042264648,0.00054407766],"genre_scores_gemma":[0.9988991,0.000026452466,0.0003360021,0.0000060160014,0.0000027229357,0.0000017825444,0.00060421805,0.0000089741225,0.00011465185],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999436,0.0000039835413,0.0000031213965,0.000019762781,0.00001751652,0.000012023691],"domain_scores_gemma":[0.99977356,0.00002535607,0.000076771896,0.000032705782,0.000041018564,0.000050673778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002272866,0.00018969878,0.00016771334,0.00064118445,0.00023255861,0.00024284079,0.00022059205,0.00016723362,0.0003627268],"category_scores_gemma":[0.0004211704,0.00011266226,0.00024118059,0.00026708707,0.00014768617,0.00022345792,0.00025299448,0.00014011623,0.00026464756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013407264,0.00003457736,0.96009135,0.000020537305,0.00005246811,0.00015344788,0.00026396732,0.0027378034,0.028354583,0.00021455581,0.000295945,0.0076467507],"study_design_scores_gemma":[0.0000024667136,0.000025972307,0.99532145,0.0000033612666,0.0000104284345,0.000052316263,0.000043402695,0.002584723,0.0015140198,0.000053346477,0.00038610096,0.00000242773],"about_ca_topic_score_codex":0.007443157,"about_ca_topic_score_gemma":0.009756459,"teacher_disagreement_score":0.007443157,"about_ca_system_score_codex":0.00039673308,"about_ca_system_score_gemma":0.00010312572,"threshold_uncertainty_score":0.0147996545},"labels":[],"label_agreement":null},{"id":"W3208045323","doi":"10.3847/1538-4357/ac51d4","title":"Radio Emission of Pulsars. II. Coherence Catalyzed by Cerenkov-unstable Shear Alfvén Waves","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics","score_opus":0.01000654597273163,"score_gpt":0.28404924918619395,"score_spread":0.2740427032134623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208045323","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9821748,0.0009696221,0.006966744,0.00017510308,0.000027512728,0.000011194915,0.000051666324,0.00005063184,0.009572735],"genre_scores_gemma":[0.9982998,0.00016849655,0.00048493722,0.000021888882,0.000024484618,0.000007375612,0.00004138446,0.0000133021695,0.0009382053],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999521,0.000007923402,0.0000018355254,0.000012730165,0.000010761707,0.0000147953015],"domain_scores_gemma":[0.999884,0.00003650598,0.00004059701,0.000012544026,0.0000133992235,0.0000129404625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010701413,0.00019522055,0.00008611891,0.00031073787,0.0002209832,0.00053725817,0.00015282632,0.00018305493,0.0011493328],"category_scores_gemma":[0.00042121898,0.00011233069,0.00010029958,0.00019162158,0.00042382514,0.00040600973,0.00035021364,0.00022603337,0.00017372263],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000780324,0.00013827966,0.07917519,0.00028203748,0.000091667265,0.0020359713,0.0028467018,0.011461711,0.6841203,0.15315497,0.0026527382,0.0632601],"study_design_scores_gemma":[0.00032469706,0.0015838784,0.49789762,0.00011832539,0.00014882786,0.0028406898,0.002884541,0.1250773,0.20955877,0.117418386,0.04201648,0.00013044897],"about_ca_topic_score_codex":0.00026945397,"about_ca_topic_score_gemma":0.0002315155,"teacher_disagreement_score":0.0011493328,"about_ca_system_score_codex":0.0001794845,"about_ca_system_score_gemma":0.000046379035,"threshold_uncertainty_score":0.0038448572},"labels":[],"label_agreement":null},{"id":"W3208135277","doi":"10.3847/1538-4357/ac501f","title":"Radio Emission of Pulsars. I. Slow Tearing of a Quantizing Magnetic Field","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Current sheet; Magnetic field; Pulsar; Omega; Atomic physics; Plasma; Neutron star; Condensed matter physics; Astrophysics; Magnetohydrodynamics; Quantum mechanics","score_opus":0.012176811230134756,"score_gpt":0.2986231929843467,"score_spread":0.28644638175421194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208135277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959455,0.00036192333,0.001917541,0.00004244498,0.0000037449827,0.000004100632,0.000043529053,0.000049332684,0.0016317349],"genre_scores_gemma":[0.99918526,0.00006121577,0.00032918202,0.000008796036,0.000006713648,0.000003633497,0.000039781768,0.000012226047,0.0003531397],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99996305,0.0000064081373,0.0000019725799,0.000011071931,0.000007785754,0.000009742222],"domain_scores_gemma":[0.99977905,0.00006744614,0.00008618813,0.000021068037,0.000020450323,0.000025761456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008275946,0.00024244795,0.0001330918,0.00038366157,0.00014703712,0.0004073259,0.00020197607,0.00020951539,0.000844533],"category_scores_gemma":[0.00047376513,0.00012303342,0.00011230744,0.0002198146,0.0004101952,0.00026565674,0.00023160137,0.00021961976,0.00017015074],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085483206,0.000054511052,0.08880695,0.00020250262,0.000053994445,0.0013666784,0.00083499687,0.009484439,0.85844684,0.009793808,0.0006615118,0.02943897],"study_design_scores_gemma":[0.00020523657,0.0012462565,0.6221038,0.00006463305,0.00009521078,0.0032768701,0.00089432654,0.106218055,0.24216534,0.015635354,0.007993807,0.00010106679],"about_ca_topic_score_codex":0.00031075,"about_ca_topic_score_gemma":0.00017435703,"teacher_disagreement_score":0.000844533,"about_ca_system_score_codex":0.00018811302,"about_ca_system_score_gemma":0.000040686427,"threshold_uncertainty_score":0.0028252602},"labels":[],"label_agreement":null},{"id":"W3208324124","doi":"10.3847/1538-4357/ac5e36","title":"The Simons Observatory: Galactic Science Goals and Forecasts","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"Science and Technology Facilities Council; David and Lucile Packard Foundation; Istituto Nazionale di Fisica Nucleare; European Commission; National Science Foundation; Royal Society; European Research Council; Gordon and Betty Moore Foundation; Simons Foundation; Massachusetts Institute of Technology; Alfred P. Sloan Foundation; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Milky Way; Observatory; Astronomy; Sky; Line-of-sight; Cosmic microwave background; Active galactic nucleus; Galaxy; Anisotropy; Optics","score_opus":0.016700565755566537,"score_gpt":0.2481174555205371,"score_spread":0.23141688976497057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208324124","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.090429746,0.010331747,0.012409074,0.13268569,0.0068060504,0.00062680483,0.19283865,0.007452193,0.54642],"genre_scores_gemma":[0.5520729,0.012168111,0.06093855,0.0068181315,0.0057823197,0.0007971166,0.22000574,0.0022672142,0.13915001],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99907047,0.0001443105,0.000049326052,0.000103997496,0.00046205704,0.00016987369],"domain_scores_gemma":[0.9972144,0.00026353647,0.00037900786,0.00022789047,0.0009238169,0.0009914822],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029397684,0.0009952608,0.00035965073,0.0020505707,0.0010446203,0.0040490944,0.00089012925,0.0012964945,0.016382651],"category_scores_gemma":[0.004511807,0.00030637128,0.0002550716,0.0024386179,0.0005001656,0.0020165923,0.0017954508,0.0015165862,0.0086152665],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045121514,0.00007636152,0.031297263,0.0003313411,0.000019323019,0.00022830757,0.0003997918,0.007624313,0.0020214925,0.047217313,0.8169373,0.093395956],"study_design_scores_gemma":[0.0001099213,0.000045035053,0.020732086,0.00019175094,0.000011161116,0.000037966558,0.00051732315,0.005320808,0.001066394,0.013983746,0.95793194,0.000051804836],"about_ca_topic_score_codex":0.074345514,"about_ca_topic_score_gemma":0.048000604,"teacher_disagreement_score":0.074345514,"about_ca_system_score_codex":0.0032659124,"about_ca_system_score_gemma":0.006541623,"threshold_uncertainty_score":0.1478256},"labels":[],"label_agreement":null},{"id":"W3208367086","doi":"10.3847/1538-4357/ac1745","title":"Quantifying Variability of Young Stellar Objects in the Mid-infrared Over 6 Years with the Near-Earth Object Wide-field Infrared Survey Explorer","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":86,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea","keywords":"Physics; Astrophysics; Young stellar object; Protostar; Astronomy; Accretion (finance); Stars; Brightness; Infrared; Infrared excess; Light curve; Stellar evolution; Variable star; Luminosity; Star formation; Galaxy","score_opus":0.02328970694260393,"score_gpt":0.2553262985334731,"score_spread":0.23203659159086917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208367086","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972652,0.000107422165,0.00022712185,0.000014172851,0.000003083218,0.0000056985655,0.002028711,0.0000144144915,0.00033419795],"genre_scores_gemma":[0.9939919,0.00008948873,0.0006695343,0.000018126533,0.000012568821,0.000012196325,0.0049576154,0.0000068189024,0.00024172492],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997905,0.000026157435,0.000021056187,0.00007328279,0.00004984734,0.0000391525],"domain_scores_gemma":[0.9991043,0.00008666553,0.00046878317,0.000067889494,0.000103897124,0.00016841764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005445762,0.00020679894,0.00021716185,0.0017668869,0.00019980817,0.00044345408,0.00020658076,0.00020932071,0.0005586474],"category_scores_gemma":[0.0006616542,0.00009987839,0.00031366816,0.00091263716,0.000112834496,0.00036717506,0.0005587781,0.00017849123,0.0002738971],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024871577,0.000013856074,0.9956548,0.000007866784,0.000045111443,0.00003537689,0.000060669878,0.00009706935,0.0017862275,0.000018058357,0.00013580151,0.0021203037],"study_design_scores_gemma":[4.2912302e-7,0.000006540778,0.9995746,0.0000012434364,0.000004863967,0.000030817657,0.000032121203,0.00010517743,0.00009446404,0.000004964538,0.00014397016,7.837747e-7],"about_ca_topic_score_codex":0.0015814502,"about_ca_topic_score_gemma":0.0039294227,"teacher_disagreement_score":0.0017668869,"about_ca_system_score_codex":0.00010818318,"about_ca_system_score_gemma":0.00008194237,"threshold_uncertainty_score":0.003144443},"labels":[],"label_agreement":null},{"id":"W3208519493","doi":"10.3847/1538-4357/ac33b0","title":"Clearing the Hurdle: The Mass of Globular Cluster Systems as a Function of Host Galaxy Mass","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Astrophysics; Physics; Globular cluster; Galaxy; Astronomy; Dwarf galaxy; Stellar mass; Star cluster; Star formation","score_opus":0.006459668570233795,"score_gpt":0.19571001085447187,"score_spread":0.18925034228423807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208519493","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905179,0.00062537217,0.00407262,0.0012544452,0.00001433351,0.00001463549,0.00069534185,0.00014412552,0.0026613027],"genre_scores_gemma":[0.9987709,0.000059242568,0.00039770943,0.00007775363,0.00002258026,0.0000042680977,0.00020601258,0.000030216936,0.00043125832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9982784,0.00072977284,0.000067730136,0.00049504533,0.00021732114,0.00021183833],"domain_scores_gemma":[0.9533471,0.03214473,0.0074267834,0.0033188919,0.0015035508,0.002258964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004817254,0.0003872928,0.00075034116,0.0017226354,0.000535267,0.0027891502,0.0012872706,0.0016059994,0.0030870242],"category_scores_gemma":[0.051087294,0.00041635951,0.0007584571,0.001701738,0.0015959791,0.003438233,0.0017032323,0.0012033129,0.0008832213],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002442409,0.00003818384,0.97632515,0.000038046186,0.00018682073,0.00021587402,0.0003036037,0.0100411875,0.00079749216,0.0035417185,0.0012072577,0.007060314],"study_design_scores_gemma":[0.00004295307,0.0002056828,0.8069479,0.000056399662,0.00018154783,0.0005651376,0.00097324874,0.17227733,0.0016128407,0.015359278,0.0017175617,0.00006019978],"about_ca_topic_score_codex":0.01352139,"about_ca_topic_score_gemma":0.0068351813,"teacher_disagreement_score":0.01352139,"about_ca_system_score_codex":0.0008431644,"about_ca_system_score_gemma":0.0003734836,"threshold_uncertainty_score":0.02688539},"labels":[],"label_agreement":null},{"id":"W3208687089","doi":"10.3847/1538-4357/ac21db","title":"Molecular Line Observations in Two Dusty Star-forming Galaxies at z = 6.9","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of British Columbia; Université de Montréal","funders":"Alfred P. Sloan Foundation; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Star (game theory); Line (geometry); Star formation; Luminous infrared galaxy","score_opus":0.02078073337842933,"score_gpt":0.2669979605985077,"score_spread":0.24621722722007838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208687089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995664,0.000015319212,0.00004263327,0.000007099151,9.4748725e-7,0.0000030140557,0.00012501597,0.0000053769445,0.00023414982],"genre_scores_gemma":[0.9992729,0.000011980453,0.00016765755,0.000008712366,0.0000025518805,0.0000030501549,0.00041237046,0.0000016939861,0.00011913306],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987626,0.000012935847,0.000007113573,0.00003715502,0.000033370245,0.000033074575],"domain_scores_gemma":[0.99969554,0.000026201162,0.000077311786,0.000020788051,0.000040701616,0.00013937026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001461201,0.00017612269,0.00024525463,0.0007804482,0.0004540001,0.00036573102,0.00026189676,0.00031753845,0.0006810607],"category_scores_gemma":[0.0002694288,0.00020463427,0.00018242766,0.0003819801,0.00018535047,0.0002035657,0.0005096457,0.00024203223,0.00021030394],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021590515,0.00013510663,0.9708231,0.000010113756,0.000035946017,0.00036486518,0.0005301711,0.00018865123,0.024057109,0.000073755094,0.00016066956,0.0034045484],"study_design_scores_gemma":[0.000006737553,0.000037747803,0.9985538,9.502194e-7,0.000006187493,0.00009082635,0.00010245017,0.0003223899,0.0006911385,0.000008407834,0.00017788347,0.0000013710824],"about_ca_topic_score_codex":0.007153659,"about_ca_topic_score_gemma":0.009863869,"teacher_disagreement_score":0.007153659,"about_ca_system_score_codex":0.00034748908,"about_ca_system_score_gemma":0.000068018744,"threshold_uncertainty_score":0.014224052},"labels":[],"label_agreement":null},{"id":"W3208879230","doi":"10.3847/1538-4357/ac4bd7","title":"Orbit Tomography of Binary Supermassive Black Holes with Very Long Baseline Interferometry","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"","keywords":"Physics; Astrophysics; Very-long-baseline interferometry; Orbit (dynamics); Supermassive black hole; Binary black hole; Gravitational wave; Astronomy; Black hole (networking); Orbital eccentricity; Very Long Baseline Array; Orbital period; Active galactic nucleus; Galaxy; Planet","score_opus":0.009454363902063759,"score_gpt":0.21501307568243366,"score_spread":0.2055587117803699,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3208879230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9434473,0.00039469913,0.053926896,0.000114547416,0.000018433391,0.000011786955,0.0002611804,0.0001629532,0.001662167],"genre_scores_gemma":[0.98720723,0.00005549387,0.01243765,0.000010729422,0.000015649048,0.0000035668666,0.00012701776,0.000007873783,0.00013476364],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999864,0.000037178062,0.0000050236454,0.000027381324,0.00003969703,0.000026695992],"domain_scores_gemma":[0.9996389,0.000070651884,0.00015032552,0.000052739786,0.00004582134,0.000041561365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036093447,0.00019663923,0.00016375237,0.0010752457,0.00016074572,0.00036417544,0.00023744888,0.00023504435,0.0005805063],"category_scores_gemma":[0.0008434405,0.00016141137,0.0001968422,0.00066987984,0.00019347107,0.00071942504,0.00054298504,0.00019852916,0.00010473946],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085756066,0.00014321065,0.4143626,0.00016168403,0.0004093131,0.0016043943,0.00042431266,0.05308483,0.33437636,0.011387903,0.0015882738,0.18159947],"study_design_scores_gemma":[0.000035174682,0.00019055698,0.34801352,0.00002133068,0.00010091617,0.0015004473,0.0002892269,0.61133105,0.028754205,0.0075058895,0.002207276,0.000050381175],"about_ca_topic_score_codex":0.0007643164,"about_ca_topic_score_gemma":0.0014822602,"teacher_disagreement_score":0.0010752457,"about_ca_system_score_codex":0.00018033468,"about_ca_system_score_gemma":0.00014761336,"threshold_uncertainty_score":0.0019420385},"labels":[],"label_agreement":null},{"id":"W3209393748","doi":"10.3847/1538-4357/ac32c6","title":"A Method to Characterize the Wide-angle Point-Spread Function of Astronomical Images","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Adaptive optics and wavefront sensing","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Starlight; Physics; Point spread function; Pixel; Optics; Stars; Galaxy; Galactic astronomy; Astrophysics; Astronomy; Milky Way","score_opus":0.014034020961284126,"score_gpt":0.24251256086384657,"score_spread":0.22847853990256245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209393748","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.019166565,0.000019846777,0.9797777,0.000019996773,0.000004251136,0.000018096305,0.00007278339,0.0006892912,0.00023141789],"genre_scores_gemma":[0.39027956,0.000060695947,0.60774153,0.000053861542,0.000017282317,0.00009818551,0.00045001935,0.00025684663,0.0010419068],"study_design_codex":"simulation_or_modeling","study_design_gemma":"not_applicable","domain_scores_codex":[0.99957305,0.00007585307,0.000021970522,0.00013637521,0.00016471591,0.000028171537],"domain_scores_gemma":[0.99889755,0.0003487482,0.00024614163,0.0002469813,0.00020836885,0.000052163745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081237324,0.0004071661,0.00035054184,0.0012607871,0.00028939365,0.000736783,0.0009922931,0.00068424636,0.0010737389],"category_scores_gemma":[0.0026778537,0.00038455357,0.0007323638,0.0005315459,0.00046166262,0.0010883512,0.0006797603,0.00054421223,0.00043478672],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013697456,0.00023902494,0.017152091,0.00009837158,0.00022907497,0.00012539512,0.0002214901,0.5364002,0.09317228,0.021830827,0.0019073839,0.32848695],"study_design_scores_gemma":[0.000004239079,0.000010960408,0.0024921934,0.0000031222953,0.0000055386217,0.000046231547,0.000007571365,0.9873762,0.0072989333,0.0019802088,0.00076098123,0.000013827809],"about_ca_topic_score_codex":0.005295298,"about_ca_topic_score_gemma":0.0049241856,"teacher_disagreement_score":0.005295298,"about_ca_system_score_codex":0.0007469673,"about_ca_system_score_gemma":0.0008364788,"threshold_uncertainty_score":0.010528982},"labels":[],"label_agreement":null},{"id":"W3209535984","doi":"10.3847/1538-4357/ac1acc","title":"The Role of Dust, UV Luminosity and Large-scale Environment on the Escape of Lyα Photons: A Case Study of a Protocluster Field at z = 3.1","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Purdue University","keywords":"Physics; Astrophysics; Galaxy; Photon; Flux (metallurgy); Luminosity; Halo; Interstellar medium; Attenuation; Optics","score_opus":0.006025635791564771,"score_gpt":0.2026118514526721,"score_spread":0.19658621566110734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209535984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99967706,0.000039047794,0.00009230223,0.000009784336,2.6946404e-7,0.0000016858812,0.000039839855,0.00000287538,0.00013718044],"genre_scores_gemma":[0.99967444,0.000037708334,0.00014544981,0.000004869559,0.0000016744729,8.574518e-7,0.000059359925,0.0000017188308,0.00007383454],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998952,0.000018397857,0.0000037012367,0.000023863857,0.000024881238,0.00003395748],"domain_scores_gemma":[0.99913627,0.00029726714,0.00023298367,0.00006754499,0.00011181867,0.00015412208],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030796527,0.00023608067,0.00021484944,0.001056096,0.0005200169,0.00051665504,0.00036345236,0.00019400624,0.00051464135],"category_scores_gemma":[0.00064395776,0.00006355776,0.00016089783,0.00057938474,0.00043883736,0.00030237608,0.000447036,0.00012991705,0.00011111533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014556179,0.000046722384,0.98205423,0.000013214748,0.000026184698,0.0017486449,0.00058714184,0.000873589,0.007430256,0.00018677318,0.00012412292,0.006763606],"study_design_scores_gemma":[0.0000033226909,0.000053538286,0.9937209,0.0000059466793,0.0000150722335,0.0006969982,0.00068479194,0.0028257044,0.0015323187,0.00013136116,0.00032345814,0.0000064160013],"about_ca_topic_score_codex":0.018165546,"about_ca_topic_score_gemma":0.016906012,"teacher_disagreement_score":0.018165546,"about_ca_system_score_codex":0.00054823485,"about_ca_system_score_gemma":0.0001461891,"threshold_uncertainty_score":0.03611964},"labels":[],"label_agreement":null},{"id":"W3209549095","doi":"10.3847/1538-4357/ac6cee","title":"Multiband Detection of Repeating FRB 20180916B","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; McGill University","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Bundesministerium für Bildung, Wissenschaft und Forschung; University of Namibia; National Commission on Research, Science and Technology; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Centre National de la Recherche Scientifique; Narodowym Centrum Nauki; Bundesministerium für Bildung und Forschung; Knut och Alice Wallenbergs Stiftelse; Science and Technology Facilities Council; National Research Foundation; Deutsche Forschungsgemeinschaft; Austrian Science Fund; Alexander von Humboldt-Stiftung","keywords":"Physics; Giant Metrewave Radio Telescope; Astrophysics; Radio telescope; Bandwidth (computing); Radio spectrum; Telescope; Range (aeronautics); Green Bank Telescope; Astronomy; Pulsar; Telecommunications; Galaxy; Radio galaxy","score_opus":0.00911204478212036,"score_gpt":0.22146902959961168,"score_spread":0.21235698481749132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209549095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971481,0.00020583325,0.0006155959,0.00004187359,0.000012451546,0.000010538465,0.00050205464,0.00005571362,0.0014078759],"genre_scores_gemma":[0.99703896,0.000062149426,0.00111493,0.00002684274,0.00002072623,0.000011366809,0.0011731876,0.000023492166,0.0005284692],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998209,0.000008842301,0.000009853225,0.000053393433,0.000062738305,0.000044313452],"domain_scores_gemma":[0.99911886,0.00007608966,0.00031736153,0.00010078003,0.00014855595,0.00023835404],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030126335,0.0003161803,0.00040960044,0.0018620844,0.0006130797,0.0005551624,0.00044995858,0.0004619193,0.0014016591],"category_scores_gemma":[0.00063801615,0.00022256677,0.00025171592,0.00089695427,0.00026071386,0.00025089597,0.00060126634,0.00042311812,0.00057494483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006997159,0.00019864838,0.68377024,0.000080281796,0.00013457537,0.0011613931,0.00059578975,0.00052622956,0.2781209,0.0003170961,0.0011502398,0.03324497],"study_design_scores_gemma":[0.000012577303,0.00014826703,0.9902124,0.000014774443,0.000027147575,0.00093141,0.00011209771,0.0006103427,0.0054435376,0.000105166146,0.0023693421,0.000012902325],"about_ca_topic_score_codex":0.0041053356,"about_ca_topic_score_gemma":0.0073739225,"teacher_disagreement_score":0.0041053356,"about_ca_system_score_codex":0.00044033607,"about_ca_system_score_gemma":0.00015480115,"threshold_uncertainty_score":0.008162856},"labels":[],"label_agreement":null},{"id":"W3209600452","doi":"10.3847/1538-4357/ac4164","title":"Optimizing the Third Generation of Gravitational-wave Observatories for Galactic Astrophysics","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; MathWorks","keywords":"Physics; Astrophysics; Astronomy; Observatory; Galaxy; Einstein Telescope; Galactic Center; Population; Sky; Gravitational wave; Supernova","score_opus":0.04841108899094468,"score_gpt":0.3171336185335204,"score_spread":0.2687225295425757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209600452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8349929,0.0006969001,0.14679009,0.001425948,0.00019255071,0.00037152358,0.0019668504,0.006800262,0.006763077],"genre_scores_gemma":[0.9337114,0.00012858833,0.062972076,0.00011856171,0.000042644584,0.00012161269,0.0018553507,0.00012789015,0.0009218757],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9981294,0.0005720074,0.0000817186,0.000387972,0.00032387816,0.00050501723],"domain_scores_gemma":[0.9869076,0.0031225507,0.0013611778,0.003468146,0.0035565381,0.0015839551],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0047193724,0.000854103,0.0008347398,0.0011446194,0.00078293314,0.0022200623,0.0016797179,0.00095656456,0.0036941725],"category_scores_gemma":[0.016507572,0.00031047076,0.00069352414,0.0011212224,0.0005550925,0.004043124,0.0022209743,0.0009769524,0.0013707549],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025030817,0.0009915703,0.4425228,0.00027992632,0.00038210012,0.00031100627,0.00032625208,0.26039538,0.0300268,0.011119676,0.019860515,0.23128095],"study_design_scores_gemma":[0.00033087906,0.000902805,0.06918331,0.00007550843,0.00018814053,0.00026557385,0.0005043011,0.89112,0.020605352,0.0061267735,0.010611269,0.00008620398],"about_ca_topic_score_codex":0.016962092,"about_ca_topic_score_gemma":0.01621154,"teacher_disagreement_score":0.016962092,"about_ca_system_score_codex":0.0015372318,"about_ca_system_score_gemma":0.0025428243,"threshold_uncertainty_score":0.033726692},"labels":[],"label_agreement":null},{"id":"W3209755171","doi":"10.3847/1538-4357/ac366a","title":"Characterization of Two 2 mm detected Optically Obscured Dusty Star-forming Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Institutes of Natural Sciences; Max-Planck-Gesellschaft; Knut och Alice Wallenbergs Stiftelse; National Research Foundation; Ministero dell’Istruzione, dell’Università e della Ricerca; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Comisión Nacional de Investigación Científica y Tecnológica; Associated Universities; National Radio Astronomy Observatory; National Astronomical Observatory of Japan; Danmarks Grundforskningsfond; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Villum Fonden; Research Corporation for Science Advancement; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Star (game theory); Star formation","score_opus":0.00746676922661097,"score_gpt":0.20827858738590044,"score_spread":0.20081181815928947,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209755171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986737,0.00005467949,0.00037298116,0.000015044965,0.0000021010123,0.0000072784756,0.00016916565,0.000027510865,0.0006775602],"genre_scores_gemma":[0.9990796,0.000010571987,0.0005190432,0.000011974012,0.0000048301104,0.0000042515103,0.00025837624,0.0000032600135,0.00010815282],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997434,0.000033892862,0.000019190911,0.000073601375,0.00006615781,0.00006372184],"domain_scores_gemma":[0.9988852,0.00014978189,0.00040623406,0.00011885969,0.00012724692,0.00031251542],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003604457,0.00025349812,0.00019892823,0.0019489096,0.00031812114,0.0007383199,0.0004090212,0.00027514528,0.0010539356],"category_scores_gemma":[0.00090882345,0.00016480753,0.00021410995,0.00053294684,0.00027385532,0.00021861862,0.0006181069,0.0001882623,0.0003006373],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000076057186,0.000028096192,0.9868362,0.000008217554,0.000016109456,0.0001848092,0.0002125634,0.0000586807,0.009200004,0.00017416722,0.00012840607,0.0030766423],"study_design_scores_gemma":[0.0000035469952,0.000028582854,0.99751425,0.0000029320047,0.000008734486,0.00025257704,0.00013964268,0.00034880106,0.0012304622,0.000048056543,0.00042010468,0.0000023417572],"about_ca_topic_score_codex":0.0027668432,"about_ca_topic_score_gemma":0.003857798,"teacher_disagreement_score":0.0027668432,"about_ca_system_score_codex":0.00031644627,"about_ca_system_score_gemma":0.00009305759,"threshold_uncertainty_score":0.0055015087},"labels":[],"label_agreement":null},{"id":"W3209897862","doi":"10.3847/1538-4357/ac562f","title":"A Simulation-based Method for Correcting Mode Coupling in CMB Angular Power Spectra","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Fermilab; British Antarctic Survey; British Columbia Knowledge Development Fund; Office of Science; Norges Forskningsråd; Vetenskapsrådet; Science and Technology Facilities Council; University of Toronto; Nuclear Safety and Security Commission; Canadian Space Agency; Inyuvesi Yakwazulu-Natali; UK Research and Innovation; National Science Foundation; Compute Canada; University of Texas at Austin; U.S. Department of Energy; Princeton University; Science Mission Directorate; Government of Ontario; National Aeronautics and Space Administration; Swedish National Space Agency","keywords":"Cosmic microwave background; Spectral line; Spectral density; Algorithm; Context (archaeology); Physics; Computational physics; Computer science; Optics; Telecommunications; Geology; Quantum mechanics","score_opus":0.01395180783204659,"score_gpt":0.28914184274182636,"score_spread":0.2751900349097798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209897862","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.008213864,0.000021157737,0.9878079,0.000055381508,0.0000320879,0.00003537595,0.000052571206,0.0019088719,0.0018727528],"genre_scores_gemma":[0.35320848,0.000075917225,0.6400156,0.000116242496,0.000040677904,0.00020223483,0.0003018122,0.001377545,0.00466139],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997414,0.00007194303,0.0000115096445,0.000034618464,0.00011451534,0.000025944062],"domain_scores_gemma":[0.99888664,0.00048361416,0.000105713625,0.00014211885,0.0003260693,0.00005580421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00073123013,0.0007730438,0.00040473993,0.0008682353,0.0006125324,0.00078330847,0.0013290403,0.00088422466,0.005116787],"category_scores_gemma":[0.0029802506,0.0005318753,0.0006339382,0.00050687697,0.00043879784,0.00056476437,0.0007115975,0.0008018891,0.0010064187],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005868398,0.000049072954,0.0010975187,0.00003826116,0.000035549227,0.00009480173,0.000069857764,0.94668585,0.008121987,0.0150863,0.001307985,0.027354186],"study_design_scores_gemma":[0.000003066835,0.0000031584104,0.000035367142,0.0000021331332,0.0000015369642,0.0000059834383,0.000002263487,0.99792117,0.00073891104,0.0007782504,0.0005057408,0.0000024093683],"about_ca_topic_score_codex":0.009258088,"about_ca_topic_score_gemma":0.006342199,"teacher_disagreement_score":0.009258088,"about_ca_system_score_codex":0.0009132849,"about_ca_system_score_gemma":0.0014546065,"threshold_uncertainty_score":0.018408418},"labels":[],"label_agreement":null},{"id":"W3209927557","doi":"10.3847/1538-4357/ac3ede","title":"Dynamical Tidal Love Numbers of Rapidly Rotating Planets and Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Canadian Institute for Theoretical Astrophysics; Alfred P. Sloan Foundation","keywords":"Physics; Dissipative system; Tidal acceleration; Rotation (mathematics); Stars; Classical mechanics; Tidal force; Astrophysics; Planet; Quantum electrodynamics; Quantum mechanics; Geometry","score_opus":0.006827022589432064,"score_gpt":0.21347984970860606,"score_spread":0.206652827119174,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3209927557","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969811,0.000024094794,0.0015832954,0.0000111218005,0.0000019645192,0.000002322646,0.00004589724,0.000020909656,0.0013291747],"genre_scores_gemma":[0.9991374,0.000013876508,0.00037919177,0.0000021523194,0.000001129635,0.0000019218928,0.00005458814,0.000008198774,0.00040152625],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992466,0.000010988428,0.0000052736327,0.000016658605,0.000023574408,0.00001880724],"domain_scores_gemma":[0.9996333,0.000098484976,0.000092606344,0.00005267837,0.00004778477,0.00007511186],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019497666,0.00018003091,0.00014860109,0.00046030545,0.00020183882,0.0004317879,0.0002335922,0.00015593432,0.0013336977],"category_scores_gemma":[0.0013975445,0.0001580391,0.00020970468,0.00021850692,0.0002631766,0.00038448002,0.00043376483,0.00016674418,0.00021049875],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004561319,0.00008312461,0.49882746,0.00011714839,0.00009913415,0.00050892227,0.00096609554,0.2770153,0.1670618,0.02054034,0.00069718034,0.033627454],"study_design_scores_gemma":[0.000015721811,0.00012587282,0.32985264,0.00001707928,0.000015589007,0.0003151549,0.00021806598,0.63312036,0.029204497,0.0053776354,0.0016867997,0.000050657105],"about_ca_topic_score_codex":0.00096398813,"about_ca_topic_score_gemma":0.0009849055,"teacher_disagreement_score":0.0013336977,"about_ca_system_score_codex":0.00024561243,"about_ca_system_score_gemma":0.00010531773,"threshold_uncertainty_score":0.004461646},"labels":[],"label_agreement":null},{"id":"W3210374197","doi":"10.3847/1538-4357/ac3e63","title":"Circumstellar Interaction Powers the Light Curves of Luminous Rapidly Evolving Optical Transients","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"National Science Foundation","keywords":"Light curve; Physics; Ejecta; Supernova; Astrophysics; Brightness; Luminosity; Observatory; Approx; Type (biology); Astronomy; Galaxy; Geology","score_opus":0.009040984896502997,"score_gpt":0.22618781945865146,"score_spread":0.21714683456214848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210374197","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99425995,0.000026850761,0.0035990754,0.000017569235,0.0000015976748,0.0000035052321,0.00012974792,0.00004849347,0.0019133895],"genre_scores_gemma":[0.99924135,0.000020567479,0.0003463435,0.0000023596983,0.0000012880628,0.0000016045511,0.00010183044,0.0000106471825,0.00027409266],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.99995005,0.000007646468,0.0000026271855,0.000016070688,0.000009414336,0.000014172732],"domain_scores_gemma":[0.999778,0.000050394003,0.00007729235,0.000036145968,0.00002643696,0.000031707048],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001459786,0.00021986992,0.00016233252,0.0004785027,0.00024727578,0.00076346577,0.00041046648,0.0002137263,0.0015961522],"category_scores_gemma":[0.00054764445,0.00016533796,0.00048736742,0.00029175228,0.0002160866,0.00042998043,0.000300916,0.00017602145,0.00021051563],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019753067,0.00010796612,0.55729806,0.00006206326,0.00013163249,0.0004637228,0.00022591995,0.36403388,0.04809091,0.008827748,0.0005730973,0.01998736],"study_design_scores_gemma":[0.000014863066,0.000078395155,0.28614777,0.000010343735,0.00004332522,0.00032613103,0.000118902084,0.7022394,0.005953715,0.0037337034,0.0013144315,0.000019011148],"about_ca_topic_score_codex":0.009085093,"about_ca_topic_score_gemma":0.006415306,"teacher_disagreement_score":0.009085093,"about_ca_system_score_codex":0.00071538036,"about_ca_system_score_gemma":0.0002490026,"threshold_uncertainty_score":0.01806444},"labels":[],"label_agreement":null},{"id":"W3210405928","doi":"10.3847/1538-4357/ac32bd","title":"Variability and Spectral Characteristics of Three Flaring Gamma-Ray Quasars Observed by VERITAS and Fermi-LAT","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Goddard Space Flight Center; Sorbonne Université; Nuclear Safety and Security Commission; Barnard College; National Aeronautics and Space Administration; U.S. Department of Energy; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Physics; Blazar; Fermi Gamma-ray Space Telescope; Astrophysics; Quasar; Gamma ray; Accretion (finance); Astronomy; Spectral energy distribution; Flare; Flux (metallurgy); Galaxy","score_opus":0.013085678206896193,"score_gpt":0.20396299619554642,"score_spread":0.19087731798865024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210405928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996026,0.00001078884,0.000053498843,0.000004473123,5.766564e-7,0.0000012926037,0.0001783946,0.000007682992,0.00014067859],"genre_scores_gemma":[0.99934953,0.0000053607623,0.0000727951,0.00000287636,0.000001152474,0.0000014801404,0.0005186757,0.0000018923216,0.000046242487],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983966,0.000018917237,0.000011942791,0.00005609479,0.000033190085,0.000040212435],"domain_scores_gemma":[0.998835,0.00024142374,0.0005407498,0.00009464393,0.00012225263,0.00016591513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004281805,0.00018082917,0.0001809658,0.0012375406,0.00027278718,0.00047532615,0.0003869208,0.0002802978,0.0006534194],"category_scores_gemma":[0.00093002093,0.00013664764,0.00024016702,0.00068964803,0.00027164625,0.00022750798,0.00040282204,0.00018488309,0.00009694525],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013105579,0.000035082066,0.99128515,0.0000048570328,0.0000454646,0.00008091519,0.00022483882,0.0007354618,0.0039217356,0.000082027094,0.00012116265,0.003332167],"study_design_scores_gemma":[0.0000043258187,0.000026115758,0.9982975,0.0000017065917,0.000009556579,0.00003563958,0.000058652964,0.0012016108,0.00024015331,0.000016335282,0.00010542271,0.0000028531203],"about_ca_topic_score_codex":0.021912135,"about_ca_topic_score_gemma":0.028506525,"teacher_disagreement_score":0.021912135,"about_ca_system_score_codex":0.0006553056,"about_ca_system_score_gemma":0.00015073777,"threshold_uncertainty_score":0.043569148},"labels":[],"label_agreement":null},{"id":"W3210528319","doi":"10.3847/1538-4357/acb53f","title":"Atmospheric Pressure and Molecular Cloud Formation in Early-type Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Flatiron Health","keywords":"Physics; Astrophysics; Molecular cloud; Atmospheric pressure; Galaxy; Hydrogen; Hydrogen molecule; Cluster (spacecraft); Galaxy cluster; Astronomy; Atomic physics; Stars; Meteorology; Quantum mechanics","score_opus":0.005873080915908383,"score_gpt":0.20500737609335656,"score_spread":0.19913429517744818,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210528319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992029,0.00015387434,0.000025082021,0.000036808073,0.0000022179634,0.0000013520178,0.00009230501,0.000005301715,0.0004801656],"genre_scores_gemma":[0.9997851,0.00003441392,0.000014114369,0.0000058903297,0.0000056911204,5.312238e-7,0.00007473767,8.9185386e-7,0.00007856447],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999089,0.000020773166,0.0000046127448,0.00001530336,0.000020024318,0.000030373996],"domain_scores_gemma":[0.99855834,0.00027522526,0.00040905754,0.000054765755,0.0000930565,0.00060956256],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023496058,0.00009963658,0.00017349137,0.0007081989,0.00024530373,0.0006404,0.00018309244,0.00029957006,0.0013653486],"category_scores_gemma":[0.0010281855,0.00009302016,0.0001404311,0.00057226536,0.0003041922,0.00022221052,0.00026308477,0.00036206833,0.0001864523],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000084842664,0.000029966595,0.9967894,0.0000045313477,0.000016604916,0.000058042144,0.00008232617,0.000058865273,0.0014283065,0.0000826785,0.00005749656,0.0013068409],"study_design_scores_gemma":[0.0000013914602,0.00001404923,0.9997676,6.3808994e-7,0.0000016162107,0.000022986645,0.000022230797,0.000058504753,0.000046830904,0.000021429261,0.000041904434,6.888044e-7],"about_ca_topic_score_codex":0.008100815,"about_ca_topic_score_gemma":0.0073086983,"teacher_disagreement_score":0.008100815,"about_ca_system_score_codex":0.0002908677,"about_ca_system_score_gemma":0.00012732258,"threshold_uncertainty_score":0.01610732},"labels":[],"label_agreement":null},{"id":"W3210555547","doi":"10.3847/1538-4357/ac2ebb","title":"Tracing the Ionization Structure of the Shocked Filaments of NGC 6240","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Institutes of Natural Sciences; Comisión Nacional de Investigación Científica y Tecnológica; National Astronomical Observatory of Japan; California Institute of Technology; Academia Sinica; National Research Council Canada; National Radio Astronomy Observatory; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; W. M. Keck Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Interstellar medium; Star formation; Ionization; Outflow; Molecular cloud; Astronomy; Stars","score_opus":0.0053577293097533465,"score_gpt":0.20107039118193124,"score_spread":0.1957126618721779,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210555547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991339,0.000028910628,0.000116201576,0.00000548928,4.555564e-7,0.0000015992397,0.00013065815,0.00002088048,0.0005618613],"genre_scores_gemma":[0.9990709,0.000023455288,0.00034889256,0.000007043213,0.0000010478191,0.0000017878788,0.00028129376,0.000005892541,0.00025965922],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999967,0.0000027107333,0.000001144893,0.000008532398,0.0000078451285,0.000012665543],"domain_scores_gemma":[0.9999043,0.000011056984,0.000030880605,0.0000073574442,0.000013305545,0.000033099863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000065058804,0.00016562814,0.000103826686,0.0007129945,0.0001926622,0.0002731458,0.00018310416,0.00021340964,0.0011763318],"category_scores_gemma":[0.0001814169,0.00015519503,0.00010703628,0.00034667045,0.000098560165,0.00015791558,0.00030815497,0.00011520242,0.00018925309],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034315782,0.00008782892,0.4043654,0.000050881386,0.000088903806,0.002018774,0.0016663434,0.004355475,0.5707502,0.00041483904,0.00050222053,0.015355855],"study_design_scores_gemma":[0.0000065414756,0.000054127788,0.9897378,0.000007502879,0.000012608255,0.00020429095,0.00020377882,0.0034576466,0.005388929,0.00011251824,0.00080761965,0.000006557247],"about_ca_topic_score_codex":0.011316603,"about_ca_topic_score_gemma":0.014412609,"teacher_disagreement_score":0.011316603,"about_ca_system_score_codex":0.00032908618,"about_ca_system_score_gemma":0.0000736546,"threshold_uncertainty_score":0.022501469},"labels":[],"label_agreement":null},{"id":"W3210575075","doi":"10.3847/1538-4357/ac3665","title":"Metallicity Distribution Function of the Eridanus II Ultra-faint Dwarf Galaxy from Hubble Space Telescope Narrowband Imaging","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; Agence Nationale de la Recherche; Space Telescope Science Institute; European Research Council; National Science Foundation","keywords":"Physics; Algorithm; Materials science; Computer science","score_opus":0.006749410301942012,"score_gpt":0.1966603675822007,"score_spread":0.1899109572802587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210575075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961201,0.000056857312,0.00048143952,0.00001557317,0.0000018195745,0.000002266113,0.0012623956,0.00008820405,0.0019714336],"genre_scores_gemma":[0.99492395,0.00003291007,0.000677715,0.000013525988,0.0000036551787,0.0000024651877,0.0035942134,0.000023053462,0.00072844],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991643,0.000004521369,0.0000037951215,0.00003776069,0.00002318413,0.000014362127],"domain_scores_gemma":[0.99976057,0.000022503522,0.00006784662,0.00004110473,0.000051807954,0.000056130164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017544454,0.00017594342,0.00014714511,0.0009782009,0.00011327855,0.00033787166,0.00017080666,0.00011561719,0.0010730425],"category_scores_gemma":[0.00033946164,0.000072959665,0.00011184202,0.0004174234,0.00012059732,0.00015788757,0.00023449684,0.000095874675,0.00061941554],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007195351,0.000019332036,0.95865554,0.000016383212,0.000031482105,0.00006507901,0.00016973451,0.0008868591,0.020457918,0.0002551937,0.0013924927,0.017977996],"study_design_scores_gemma":[0.0000018718309,0.000009676896,0.9955918,0.0000032957657,0.0000051793827,0.000048807473,0.00003967508,0.0011655362,0.0019039029,0.00005413526,0.0011724713,0.0000036192696],"about_ca_topic_score_codex":0.005424064,"about_ca_topic_score_gemma":0.0075835506,"teacher_disagreement_score":0.005424064,"about_ca_system_score_codex":0.0003517111,"about_ca_system_score_gemma":0.000072068266,"threshold_uncertainty_score":0.010784984},"labels":[],"label_agreement":null},{"id":"W3210582858","doi":"10.3847/1538-4357/ac332e","title":"The Variability of the Black Hole Image in M87 at the Dynamical Timescale","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Astrophysics Division; National Key Research and Development Program of China; Japan Society for the Promotion of Science; National Nuclear Security Administration; Toray Science Foundation; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Recruitment Program of Global Experts; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Natural Sciences and Engineering Research Council of Canada; European Southern Observatory; China Scholarship Council; John Templeton Foundation; Ministry of Education, Culture, Sports, Science and Technology; Ministerio de Economía y Competitividad; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Harvard University; Radboud Universiteit; National Research Foundation; Division of Biological Infrastructure; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; National Institutes of Natural Sciences; Government of Canada; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Kavli Foundation; National Astronomical Observatory of Japan; Associated Universities; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; Compute Canada; Simons Foundation; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Flatiron Health","keywords":"Physics; Astrophysics; Black hole (networking); Supermassive black hole; Galaxy; Observable; Quantum mechanics","score_opus":0.005944700372028821,"score_gpt":0.21546867282862886,"score_spread":0.20952397245660004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210582858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992823,0.00001985672,0.00033030086,0.000010531612,0.0000012953345,0.0000020989012,0.000096093245,0.000019756644,0.00023778746],"genre_scores_gemma":[0.9995964,0.000007156908,0.00013706293,0.0000022217803,0.0000013397407,0.0000013633535,0.00022397934,0.0000061948513,0.000024365567],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990153,0.000019406056,0.000004930128,0.000022749206,0.000023835484,0.000027617207],"domain_scores_gemma":[0.9995474,0.00014939699,0.00009258329,0.0000727037,0.00006324913,0.00007463594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003831022,0.00019884364,0.00026961174,0.0004235499,0.00020385045,0.0005595168,0.00036798156,0.0002637473,0.00044933747],"category_scores_gemma":[0.001329015,0.00012860143,0.00046610305,0.00029737243,0.00030320167,0.00028862982,0.00032873874,0.00023772682,0.000094281546],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077485165,0.00019624268,0.74059427,0.00007289962,0.0003364549,0.0006299308,0.00057804317,0.18798774,0.05267919,0.0022984585,0.00097133237,0.01288069],"study_design_scores_gemma":[0.000025046664,0.00010105692,0.7920718,0.000008263334,0.000040537707,0.0001089353,0.00014946684,0.20225444,0.0043975394,0.0003999372,0.00042338824,0.000019496223],"about_ca_topic_score_codex":0.0044753384,"about_ca_topic_score_gemma":0.0031548266,"teacher_disagreement_score":0.0044753384,"about_ca_system_score_codex":0.00048650807,"about_ca_system_score_gemma":0.00016115302,"threshold_uncertainty_score":0.008898556},"labels":[],"label_agreement":null},{"id":"W3210979068","doi":"10.3847/1538-4357/ac35d9","title":"The Distance and Dynamical History of the Virgo Cluster Ultradiffuse Galaxy VCC 615","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Algorithm; Physics; Computer science","score_opus":0.004483383289163554,"score_gpt":0.17884539490480922,"score_spread":0.17436201161564566,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3210979068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99802655,0.00010344562,0.00010672588,0.00003823949,0.000003339864,0.0000028932907,0.0003476342,0.000014017798,0.0013571015],"genre_scores_gemma":[0.9986247,0.000022718683,0.000143454,0.000017300696,0.0000020468901,0.0000020356224,0.0008218524,0.0000050109966,0.0003609947],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998517,0.000008701258,0.000004562676,0.000050304418,0.000046583027,0.000038148497],"domain_scores_gemma":[0.99959165,0.000037777452,0.000071857525,0.000045652603,0.000071009454,0.00018207809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019170475,0.00012871235,0.0001637683,0.0009618707,0.0005211843,0.0006494488,0.00031374893,0.00020676917,0.0014475432],"category_scores_gemma":[0.00087574305,0.00010716823,0.00014870783,0.0005322077,0.0002900906,0.0002698993,0.00077928696,0.00020883848,0.00032909718],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008155055,0.00003298615,0.97481936,0.000023587296,0.00004744885,0.00016209712,0.00044279167,0.0021332302,0.008277193,0.001241892,0.0015249611,0.011212912],"study_design_scores_gemma":[0.000003233552,0.0000150002525,0.99464464,0.0000068547583,0.000006883865,0.000058980884,0.00012755895,0.0025388699,0.0005569317,0.00015821327,0.0018748351,0.000008046488],"about_ca_topic_score_codex":0.039714087,"about_ca_topic_score_gemma":0.035130516,"teacher_disagreement_score":0.039714087,"about_ca_system_score_codex":0.0014182343,"about_ca_system_score_gemma":0.00020915233,"threshold_uncertainty_score":0.07896584},"labels":[],"label_agreement":null},{"id":"W3211237148","doi":"10.3847/1538-4357/ac1353","title":"Very Large Telescope Spectroscopy of Ultra-faint Dwarf Galaxies. I. Boötes I, Leo IV, and Leo V","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics","score_opus":0.008113343401843203,"score_gpt":0.22521010999029373,"score_spread":0.21709676658845053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3211237148","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932632,0.0003368421,0.0011273391,0.00007560541,0.000013145784,0.00001661499,0.0008533205,0.0001251443,0.0041887783],"genre_scores_gemma":[0.99240196,0.00009703747,0.0026012287,0.00007272798,0.000020229332,0.000018759369,0.0028935801,0.00004276293,0.0018516607],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99964535,0.00003720739,0.000014836225,0.00010198397,0.00010367855,0.000096943826],"domain_scores_gemma":[0.999311,0.00006974531,0.00013622326,0.0001411931,0.00009003163,0.00025174933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005631807,0.0002589446,0.00025474324,0.0013700468,0.00046248676,0.0005684591,0.00046071527,0.0002004025,0.0009684764],"category_scores_gemma":[0.0006129698,0.00018475267,0.00023844872,0.00068853126,0.00030740528,0.00027894857,0.0010307162,0.00026442963,0.000444897],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026167757,0.00014760875,0.88886684,0.000066723296,0.00009350436,0.00032490268,0.00081620144,0.00064676075,0.061282743,0.0014381984,0.003020772,0.04303411],"study_design_scores_gemma":[0.000023075507,0.000056286754,0.9859228,0.000011457846,0.000023710707,0.0001137028,0.0002459975,0.00064126885,0.0040623765,0.00020263474,0.008687827,0.000008881583],"about_ca_topic_score_codex":0.005926416,"about_ca_topic_score_gemma":0.015951792,"teacher_disagreement_score":0.005926416,"about_ca_system_score_codex":0.0007174969,"about_ca_system_score_gemma":0.00023673815,"threshold_uncertainty_score":0.011783898},"labels":[],"label_agreement":null},{"id":"W3211276979","doi":"10.3847/1538-4357/ac1869","title":"Kinematics of Antlia 2 and Crater 2 from the Southern Stellar Stream Spectroscopic Survey (S <sup>5</sup>)","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":94,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"European Space Agency; National Aeronautics and Space Administration; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Milky Way; Astrophysics; Galaxy; Stellar kinematics; Astronomy; Dwarf galaxy; Metallicity; Local Group; Stars","score_opus":0.013140439569911275,"score_gpt":0.22391364464980798,"score_spread":0.21077320507989672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3211276979","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997437,0.0000553738,0.00009736596,0.00002986617,0.000002647928,0.00000902445,0.0006952183,0.000025031177,0.0016485009],"genre_scores_gemma":[0.99443674,0.00006031528,0.0010336791,0.000030700096,0.000007420112,0.000009266547,0.0033647756,0.000012280535,0.0010446991],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982786,0.000014718317,0.000008025306,0.00006276801,0.000054960612,0.000031725387],"domain_scores_gemma":[0.99954176,0.000020635678,0.00017442225,0.000049455608,0.000083396946,0.0001303501],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018763132,0.000244227,0.00019657212,0.0011824724,0.00031516637,0.00048989867,0.00027880102,0.0001899529,0.00083863444],"category_scores_gemma":[0.00039497003,0.00022088988,0.00017312814,0.0007039855,0.00021796153,0.00020261163,0.00075888046,0.00020281902,0.00037039915],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010184302,0.000030431933,0.98391336,0.0000123846285,0.000032389435,0.00019004621,0.0005042458,0.00017993574,0.0073125055,0.000107900254,0.0009717313,0.0066432455],"study_design_scores_gemma":[0.00000471464,0.00002167531,0.9974468,0.0000024479532,0.0000072505427,0.00013851358,0.00014157323,0.00028054335,0.0003149935,0.00001634981,0.0016225035,0.00000270128],"about_ca_topic_score_codex":0.034321003,"about_ca_topic_score_gemma":0.1497536,"teacher_disagreement_score":0.034321003,"about_ca_system_score_codex":0.0005273472,"about_ca_system_score_gemma":0.00029416432,"threshold_uncertainty_score":0.06824249},"labels":[],"label_agreement":null},{"id":"W3211565371","doi":"10.3847/1538-4357/ac3a89","title":"GASKAP Pilot Survey Science. II. ASKAP Zoom Observations of Galactic 21 cm Absorption","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Université Laval","funders":"","keywords":"Astrophysics; Physics; Galaxy; RADIUS; Milky Way; Surface brightness; Astronomy; Population; Galactic plane","score_opus":0.042163757649358286,"score_gpt":0.26668182456452155,"score_spread":0.22451806691516327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3211565371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.56324923,0.00039156832,0.0033859627,0.0011681298,0.00010150393,0.00045535614,0.35615313,0.0063986145,0.06869645],"genre_scores_gemma":[0.66518605,0.00029529398,0.016272774,0.0005688419,0.00011463553,0.0006374245,0.28511822,0.000810629,0.030996101],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998472,0.000026329937,0.0000047103636,0.0000360939,0.000042743453,0.000042840173],"domain_scores_gemma":[0.9995136,0.000047139572,0.00006731721,0.000113606635,0.00010684382,0.00015140756],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047319056,0.00028671845,0.00016438816,0.0014901445,0.0004137578,0.0003821003,0.00038390083,0.00020340795,0.013147898],"category_scores_gemma":[0.0004597503,0.00018631759,0.00020055658,0.0015882514,0.00013366513,0.00037485475,0.00065065,0.00021266115,0.0042497395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00249978,0.00030957174,0.49172944,0.00061303866,0.00022696563,0.0009311333,0.0011001481,0.0029840244,0.037454955,0.0026018398,0.26954448,0.19000469],"study_design_scores_gemma":[0.00013263409,0.00012730905,0.914552,0.000026777125,0.000036827605,0.00017595543,0.00026468452,0.002064859,0.0035203693,0.00048304597,0.07859242,0.000023125609],"about_ca_topic_score_codex":0.029226989,"about_ca_topic_score_gemma":0.05904548,"teacher_disagreement_score":0.029226989,"about_ca_system_score_codex":0.0004613883,"about_ca_system_score_gemma":0.00055369164,"threshold_uncertainty_score":0.058113754},"labels":[],"label_agreement":null},{"id":"W3211893519","doi":"10.3847/1538-4357/ac63c5","title":"COMAP Early Science. IV. Power Spectrum Methodology and Results","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Jet Propulsion Laboratory; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Toronto; Keck Institute for Space Studies; Norges Forskningsråd; California Institute of Technology; University of Miami; National Aeronautics and Space Administration; European Research Council; National Science Foundation","keywords":"Spectrum (functional analysis); Power (physics); Computer science; Environmental science; Physics","score_opus":0.02565555593053731,"score_gpt":0.26576317785545817,"score_spread":0.24010762192492086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3211893519","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.28569224,0.000508673,0.36722302,0.0018529483,0.00035583918,0.0010887193,0.13323556,0.0321914,0.17785148],"genre_scores_gemma":[0.57029605,0.00045094787,0.33958113,0.0006017304,0.00026495778,0.0016427326,0.05575055,0.009557275,0.021854736],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987213,0.00018578646,0.00005376348,0.00020925599,0.0006406361,0.00018919005],"domain_scores_gemma":[0.99598145,0.00074900896,0.00048533606,0.0012133854,0.0013174346,0.0002533871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002394888,0.00084418256,0.00050230295,0.005861714,0.0011908896,0.002386695,0.0014115436,0.0005436365,0.015228457],"category_scores_gemma":[0.006954032,0.00037307918,0.0007332947,0.005850687,0.00053030986,0.0009687463,0.0016792637,0.0010760075,0.006013019],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005873514,0.00041732466,0.17529681,0.0012913095,0.0006023148,0.001351035,0.0012793808,0.025692962,0.026507976,0.12275416,0.18219686,0.4620225],"study_design_scores_gemma":[0.00012058726,0.00020789681,0.3864772,0.00019521923,0.00015271697,0.0010812909,0.0007239239,0.11825601,0.041167688,0.06176771,0.3896793,0.00017050479],"about_ca_topic_score_codex":0.006694703,"about_ca_topic_score_gemma":0.0050932053,"teacher_disagreement_score":0.015228457,"about_ca_system_score_codex":0.0009388788,"about_ca_system_score_gemma":0.0009886152,"threshold_uncertainty_score":0.05094427},"labels":[],"label_agreement":null},{"id":"W3211947425","doi":"10.3847/1538-4357/ac517c","title":"Selection Effects in Periodic X-Ray Data from Maximizing Detection Statistics","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"National Science Foundation","keywords":"Amplitude; Algorithm; Statistics; Computer science; Physics; Mathematics; Optics","score_opus":0.017165417534654143,"score_gpt":0.3072065956218137,"score_spread":0.29004117808715957,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3211947425","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6260387,0.0007410788,0.35890543,0.0025201545,0.00016707579,0.00031350923,0.00091363204,0.000935499,0.009465006],"genre_scores_gemma":[0.9105785,0.00010452942,0.08688775,0.0005862404,0.00010462008,0.00019119852,0.0007162895,0.00020650985,0.00062433566],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9524597,0.036274165,0.0019185984,0.0037750038,0.004751349,0.0008210922],"domain_scores_gemma":[0.7013788,0.2591071,0.012807179,0.020033056,0.0052306685,0.0014431193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.058093492,0.00056612625,0.0011619676,0.0014976114,0.00091853837,0.0026059675,0.0018192952,0.0012721391,0.0013896438],"category_scores_gemma":[0.25489822,0.0006338288,0.0009194289,0.0016884868,0.0027739187,0.0023627868,0.0026317765,0.0016091579,0.00032772173],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025250767,0.00027233505,0.52563775,0.0006026014,0.0014220471,0.0015741077,0.0026136811,0.0895139,0.013609432,0.09238194,0.011840831,0.25800627],"study_design_scores_gemma":[0.00042577105,0.00085426366,0.21488953,0.0002844579,0.00044737683,0.001698068,0.0007618218,0.5129287,0.026611455,0.23195441,0.008905321,0.00023879105],"about_ca_topic_score_codex":0.0015993584,"about_ca_topic_score_gemma":0.0015784123,"teacher_disagreement_score":0.058093492,"about_ca_system_score_codex":0.0011601119,"about_ca_system_score_gemma":0.0012870358,"threshold_uncertainty_score":0.30723143},"labels":[],"label_agreement":null},{"id":"W3212783471","doi":"10.3847/1538-4357/ac36d2","title":"The VLA/ALMA Nascent Disk And Multiplicity (VANDAM) Survey of Orion Protostars. V. A Characterization of Protostellar Multiplicity","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Instituto de Astrofísica de Andalucía; Fondo Nacional de Desarrollo Científico y Tecnológico; National Astronomical Observatory of Japan; National Science Council; Nuclear Safety and Security Commission; Ministerio de Ciencia, Innovación y Universidades; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Agencia Estatal de Investigación; National Radio Astronomy Observatory; Centro de Astrofísica y Tecnologías Afines; Space Telescope Science Institute; Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España; National Science Foundation","keywords":"Protostar; Physics; Astrophysics; Stars; Star formation; Multiplicity (mathematics); Molecular cloud; Astronomy; Geometry","score_opus":0.01295648441650352,"score_gpt":0.23812098537053777,"score_spread":0.22516450095403426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3212783471","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990409,0.00006138188,0.000070838876,0.000009030673,0.0000010878261,0.0000022285374,0.00032422369,0.000006269608,0.00048401806],"genre_scores_gemma":[0.9975739,0.00003360689,0.0005749075,0.000008276453,0.0000045182255,0.000006234562,0.001293244,0.0000038074277,0.00050148193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988294,0.000018700186,0.0000072790654,0.000034487923,0.000031607062,0.000025016529],"domain_scores_gemma":[0.9996828,0.000034001132,0.00012185591,0.000030567146,0.000036484817,0.00009423895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018107954,0.00012499701,0.00009687714,0.0010552473,0.0002520925,0.00037996442,0.00019585463,0.00013529263,0.0006809238],"category_scores_gemma":[0.00055823487,0.0000839588,0.00009788206,0.00036618803,0.000150245,0.00020883112,0.00039428048,0.00010675403,0.00019699842],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007543018,0.000020469515,0.97796464,0.000010844789,0.00001647494,0.00009879327,0.00026073307,0.00014670235,0.01371881,0.00018441865,0.00027661113,0.0072260792],"study_design_scores_gemma":[0.0000030698923,0.000015664195,0.9976774,0.0000027313124,0.0000031667764,0.00011608276,0.00007372269,0.00039622936,0.0006536089,0.00003951246,0.0010167644,0.0000020537607],"about_ca_topic_score_codex":0.0073980964,"about_ca_topic_score_gemma":0.014380984,"teacher_disagreement_score":0.0073980964,"about_ca_system_score_codex":0.00036894612,"about_ca_system_score_gemma":0.0001597059,"threshold_uncertainty_score":0.014710069},"labels":[],"label_agreement":null},{"id":"W3212807346","doi":"10.3847/1538-4357/ac5019","title":"GWSkyNet-Multi: A Machine-learning Multiclass Classifier for LIGO–Virgo Public Alerts","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Istituto Nazionale di Fisica Nucleare; Centre National de la Recherche Scientifique; Canada Research Chairs; Max-Planck-Gesellschaft; National Science Foundation","keywords":"LIGO; Gravitational wave; Physics; Neutron star; Binary black hole; Binary number; Classifier (UML); Binary classification; Astrophysics; Astronomy; Artificial intelligence; Computer science; Support vector machine","score_opus":0.04551384880903381,"score_gpt":0.35137568728320095,"score_spread":0.30586183847416715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3212807346","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7656513,0.0038950911,0.13390163,0.0026944687,0.0012904558,0.0008553614,0.022920193,0.05727438,0.011517178],"genre_scores_gemma":[0.87397856,0.00032595504,0.0856945,0.0007346505,0.00024931756,0.0003905843,0.031623397,0.00044770548,0.006555288],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99899393,0.00021561458,0.00009258728,0.00029752514,0.00023017485,0.00017024616],"domain_scores_gemma":[0.9980982,0.00077209354,0.0001919323,0.00033914283,0.0003782167,0.00022041038],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024482347,0.0025732778,0.0012781668,0.0034826235,0.00075623713,0.0012325541,0.0027580105,0.0031588404,0.0037788227],"category_scores_gemma":[0.004348757,0.00044708693,0.0011456911,0.0012931833,0.00051320967,0.001803181,0.0019484495,0.0021989273,0.0024728854],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017763735,0.0018505224,0.039115302,0.0004782579,0.0006084801,0.0005279715,0.00016022826,0.20689636,0.0065779374,0.0024046495,0.098443486,0.6411604],"study_design_scores_gemma":[0.000069551555,0.00018739831,0.0030310662,0.000029421208,0.00003632923,0.000056476143,0.000051242594,0.9877836,0.003492816,0.0024022718,0.0028304276,0.000029477322],"about_ca_topic_score_codex":0.010478921,"about_ca_topic_score_gemma":0.008826372,"teacher_disagreement_score":0.010478921,"about_ca_system_score_codex":0.0013356793,"about_ca_system_score_gemma":0.0012455223,"threshold_uncertainty_score":0.020835817},"labels":[],"label_agreement":null},{"id":"W3212912157","doi":"10.3847/1538-4357/ac375d","title":"Study of 72 Pulsars Discovered in the PALFA Survey: Timing Analysis, Glitch Activity, Emission Variability, and a Pulsar in an Eccentric Binary","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"Precursory Research for Embryonic Science and Technology; U.S. Naval Research Laboratory; Office of Naval Research; Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; Queens College, City University of New York; McGill Space Institute; University of British Columbia; Science and Technology Facilities Council; University of Toronto; National Science Foundation; Compute Canada; McGill University; Fondation familiale Trottier; City University of New York; Western Canada Research Grid; Canadian Institute for Advanced Research; State Key Laboratory of Automotive Simulation and Control; National Aeronautics and Space Administration","keywords":"Pulsar; Physics; Millisecond pulsar; Astrophysics; Neutron star; Galactic plane; Binary pulsar; Astronomy; Population; Pulsar planet; X-ray pulsar; Magnetosphere; Sky; Stars; Magnetic field","score_opus":0.031306116590240345,"score_gpt":0.35497896165272846,"score_spread":0.3236728450624881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3212912157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991731,0.00006690355,0.00010557366,0.000010475092,0.0000020421592,0.000002383788,0.0003120488,0.000007878719,0.00031953992],"genre_scores_gemma":[0.9981154,0.000083063154,0.00021224779,0.000008561608,0.000008836492,0.0000055885885,0.0012616547,0.000003166445,0.00030148547],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998853,0.000013114387,0.000009686335,0.000037973154,0.000025222127,0.000028679116],"domain_scores_gemma":[0.9994324,0.00007456631,0.00022542536,0.000052450043,0.00010661001,0.00010857697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002260642,0.00016425029,0.00015670103,0.0015936929,0.000352929,0.00038332833,0.00018132332,0.00014202703,0.00072677876],"category_scores_gemma":[0.000458046,0.00007846737,0.00013294962,0.0010277036,0.00019611308,0.0002335677,0.00037015715,0.00016041819,0.00025388418],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000077465076,0.000021347782,0.989583,0.000011889878,0.000016668342,0.00024128746,0.00014777906,0.000038604667,0.0041464465,0.00002093344,0.00011281867,0.0055817775],"study_design_scores_gemma":[0.0000017268084,0.000038116148,0.9985629,0.0000018570278,0.0000073601555,0.00030750417,0.00011656614,0.00008220441,0.00039085932,0.0000072173707,0.00048217457,0.0000015028662],"about_ca_topic_score_codex":0.0029709917,"about_ca_topic_score_gemma":0.0050418847,"teacher_disagreement_score":0.0029709917,"about_ca_system_score_codex":0.00018194612,"about_ca_system_score_gemma":0.00015092417,"threshold_uncertainty_score":0.0059074163},"labels":[],"label_agreement":null},{"id":"W3212956292","doi":"10.3847/1538-4357/ac3a7a","title":"The Mass of the Milky Way from the H3 Survey","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Space Telescope Science Institute","keywords":"Milky Way; Physics; Halo; Virial mass; Astrophysics; Galaxy","score_opus":0.02006223251136702,"score_gpt":0.2367875600725973,"score_spread":0.21672532756123028,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3212956292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9854768,0.00046217817,0.002316513,0.00013277361,0.0000052540327,0.0000078240455,0.008920793,0.00029391478,0.0023838691],"genre_scores_gemma":[0.98916864,0.00015988435,0.0015523806,0.00005160571,0.000012694169,0.000009612484,0.008552507,0.000101193466,0.00039152234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998323,0.00003034584,0.00000843312,0.00005857419,0.00003956783,0.000030707797],"domain_scores_gemma":[0.99898034,0.00023443204,0.00032009705,0.00017881858,0.00012552946,0.00016077972],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005653261,0.00023621845,0.00025538672,0.0009801236,0.00015301588,0.000678323,0.00034311056,0.00033393074,0.0017224409],"category_scores_gemma":[0.0017390868,0.00011533047,0.00046487214,0.001081108,0.0003625951,0.0004057598,0.0010057492,0.00027421588,0.0008740204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028747026,0.00001970584,0.95089203,0.00011051281,0.00037894325,0.00024444258,0.0004855641,0.014235819,0.006840078,0.0019759464,0.0057175253,0.018811885],"study_design_scores_gemma":[0.000022637807,0.000028464416,0.97768813,0.000035176865,0.00004769803,0.00017470909,0.00031129285,0.010250725,0.002452578,0.0016728455,0.0072893724,0.000026330907],"about_ca_topic_score_codex":0.016096402,"about_ca_topic_score_gemma":0.010114889,"teacher_disagreement_score":0.016096402,"about_ca_system_score_codex":0.00045244844,"about_ca_system_score_gemma":0.00024252124,"threshold_uncertainty_score":0.03200543},"labels":[],"label_agreement":null},{"id":"W3213082769","doi":"10.3847/1538-4357/ac382b","title":"Accretion Flows or Outflow Cavities? Uncovering the Gas Dynamics around Lupus 3-MMS","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Ministry of Science and Technology, Taiwan","keywords":"Physics; Outflow; Protostar; Accretion (finance); Astrophysics; Astronomy; Star formation; Stars","score_opus":0.010829641290753958,"score_gpt":0.23181882698172196,"score_spread":0.220989185690968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3213082769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99924695,0.000031221338,0.0002704027,0.000009583263,7.618539e-7,0.0000030236656,0.00014876471,0.000028557972,0.00026078185],"genre_scores_gemma":[0.9988951,0.000015870255,0.00076853926,0.000005267213,0.0000027999233,0.0000018250961,0.00026043484,0.0000065744107,0.00004357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999418,0.000006894874,0.0000034313825,0.000020346339,0.0000108547865,0.000016615546],"domain_scores_gemma":[0.9995185,0.000066987726,0.00020889225,0.00003239596,0.00003666622,0.00013652132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001849411,0.00018168434,0.00024206247,0.0017105843,0.00039856287,0.00053581654,0.0002731648,0.00023711045,0.0005718918],"category_scores_gemma":[0.0004470424,0.00011756889,0.00026135,0.00096495706,0.0003117961,0.00026420786,0.00043418264,0.00019691428,0.00017824699],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001655772,0.00004340519,0.9558406,0.000026852736,0.000027300226,0.0005522655,0.00054585276,0.0011423973,0.033337917,0.00027953298,0.00021518719,0.007823101],"study_design_scores_gemma":[0.000008417121,0.00006807891,0.98737735,0.000011267026,0.000019074085,0.00028004742,0.00041411046,0.008104757,0.0026776802,0.0003995561,0.00063255295,0.0000070452334],"about_ca_topic_score_codex":0.0028677722,"about_ca_topic_score_gemma":0.0038092576,"teacher_disagreement_score":0.0028677722,"about_ca_system_score_codex":0.00031160147,"about_ca_system_score_gemma":0.00014911036,"threshold_uncertainty_score":0.005702138},"labels":[],"label_agreement":null},{"id":"W3213121630","doi":"10.3847/1538-4357/ac5829","title":"Bayesian Solar Wind Modeling with Pulsar Timing Arrays","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Science and Technology Facilities Council; National Aeronautics and Space Administration","keywords":"Physics; Coronal mass ejection; Pulsar; Solar wind; Solar cycle; Solar physics; Solar maximum; Computational physics; Astrophysics; Astronomy; Remote sensing; Plasma","score_opus":0.009565188093823921,"score_gpt":0.2144821727533539,"score_spread":0.20491698465952998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3213121630","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.25381374,0.00014102571,0.7399427,0.0004149045,0.00004051304,0.000030287008,0.0006776775,0.0005796435,0.004359446],"genre_scores_gemma":[0.936834,0.000114124865,0.059760474,0.00007306555,0.000050628987,0.000050753468,0.00071116944,0.00016726354,0.0022386597],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996853,0.00014010204,0.000013331841,0.00007443879,0.000064660715,0.000022162647],"domain_scores_gemma":[0.99810153,0.0011523557,0.00034659173,0.0001411495,0.00019567144,0.00006265521],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001466844,0.00038537523,0.00043958158,0.00063151034,0.00040019388,0.0010642451,0.00072673056,0.0005420085,0.0017985762],"category_scores_gemma":[0.0072121304,0.00041672008,0.00061776355,0.0007614909,0.00041577112,0.0010093364,0.00062918355,0.0009944584,0.0002851118],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000025321917,0.0000130830385,0.0046541705,0.000006845984,0.000032610904,0.000022925522,0.000027058526,0.977896,0.00045925175,0.010934762,0.0002701654,0.0056577437],"study_design_scores_gemma":[0.000002312843,0.0000031740847,0.00061205425,0.0000019358893,0.0000022285028,0.000004032282,0.0000037108418,0.9948907,0.000068896836,0.0042295186,0.00017766905,0.0000037568227],"about_ca_topic_score_codex":0.011424337,"about_ca_topic_score_gemma":0.011411554,"teacher_disagreement_score":0.011424337,"about_ca_system_score_codex":0.00060599047,"about_ca_system_score_gemma":0.00059200736,"threshold_uncertainty_score":0.022715688},"labels":[],"label_agreement":null},{"id":"W3213977292","doi":"10.3847/1538-4357/ac63ca","title":"COMAP Early Science. III. CO Data Processing","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Jet Propulsion Laboratory; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Toronto; Keck Institute for Space Studies; Norges Forskningsråd; California Institute of Technology; University of Miami; National Aeronautics and Space Administration; European Research Council; National Science Foundation","keywords":"Calibration; Noise (video); Lissajous curve; Pipeline (software); Spectral density; Detector; Residual; Computer science; Data processing; Statistics; Algorithm; Remote sensing; Mathematics; Artificial intelligence; Physics; Optics; Geography","score_opus":0.025182333439917708,"score_gpt":0.2756282109315959,"score_spread":0.2504458774916782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3213977292","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.017395766,0.00036054527,0.12671065,0.001349347,0.0007829108,0.0010542091,0.4275843,0.2926477,0.1321146],"genre_scores_gemma":[0.09843591,0.00039848828,0.2964379,0.0014039857,0.0006086442,0.0028159332,0.4603556,0.086347066,0.053196482],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.998667,0.00013842735,0.00009634817,0.00039379636,0.00049488235,0.00020955974],"domain_scores_gemma":[0.994177,0.0006317444,0.0005276834,0.0018649306,0.0023044087,0.00049429556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018921396,0.0011524239,0.0009355088,0.004619051,0.0012540915,0.0041762725,0.0021025725,0.00080479606,0.08877717],"category_scores_gemma":[0.0076568476,0.00085513026,0.0008842002,0.0069342568,0.00047659152,0.001696668,0.0023527548,0.001736197,0.088139825],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007350403,0.00011093047,0.01369945,0.0006833332,0.0001664003,0.00033056852,0.00033713243,0.0024364032,0.009195153,0.007094791,0.7745134,0.19069742],"study_design_scores_gemma":[0.00013813646,0.00007642375,0.029673317,0.00013453396,0.000061051076,0.0002769064,0.00017484564,0.01906222,0.025588756,0.009826729,0.9148699,0.00011724171],"about_ca_topic_score_codex":0.006830525,"about_ca_topic_score_gemma":0.0073585603,"teacher_disagreement_score":0.08877717,"about_ca_system_score_codex":0.0012063185,"about_ca_system_score_gemma":0.0025283357,"threshold_uncertainty_score":0.2969892},"labels":[],"label_agreement":null},{"id":"W3214208556","doi":"10.3847/1538-4357/ac63c9","title":"COMAP Early Science. VII. Prospects for CO Intensity Mapping at Reionization","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"European Research Council; Jet Propulsion Laboratory; Universitetet i Oslo; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; California Institute of Technology; European Commission; Science and Technology Facilities Council; University of Toronto; Keck Institute for Space Studies; Norges Forskningsråd; University of Miami; National Aeronautics and Space Administration; National Science Foundation","keywords":"Reionization; Physics; Intensity mapping; Redshift; COSMIC cancer database; Astrophysics; Galaxy; Dark Ages; Radiative transfer; Astronomy; Pathfinder; Cosmic microwave background; Optics","score_opus":0.012169445205635532,"score_gpt":0.22820597521610891,"score_spread":0.21603653001047338,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214208556","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17286901,0.023289967,0.09730764,0.20452437,0.008594915,0.0002832634,0.029742913,0.021810478,0.4415774],"genre_scores_gemma":[0.75621396,0.013133252,0.11181389,0.016936166,0.0034921863,0.0002033474,0.017109092,0.0025865568,0.07851166],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9992374,0.00015594214,0.000018000124,0.00014368283,0.00026554646,0.00017951055],"domain_scores_gemma":[0.99515945,0.0007625219,0.0005477773,0.0011172963,0.0011778041,0.0012352725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005077519,0.0007944351,0.00034000524,0.0018468774,0.0009675675,0.0034193438,0.001215296,0.0018862807,0.014186597],"category_scores_gemma":[0.0048745153,0.00035622716,0.00042016967,0.0022546365,0.0010706307,0.0033438571,0.0019754977,0.0021240169,0.0055929134],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006518437,0.00017132203,0.033959404,0.000645365,0.00010359256,0.0010912591,0.00043117735,0.008892372,0.009016466,0.25599352,0.2694139,0.4196298],"study_design_scores_gemma":[0.000060537666,0.00012853536,0.046856962,0.00021708192,0.000028579992,0.0005608885,0.0002142302,0.015174064,0.0071000564,0.114276595,0.81528336,0.000099129866],"about_ca_topic_score_codex":0.0032494166,"about_ca_topic_score_gemma":0.0029876388,"teacher_disagreement_score":0.014186597,"about_ca_system_score_codex":0.002432317,"about_ca_system_score_gemma":0.0015090673,"threshold_uncertainty_score":0.047458887},"labels":[],"label_agreement":null},{"id":"W3214217376","doi":"10.3847/1538-4357/ac6a55","title":"Improving Cosmological Constraints from Galaxy Cluster Number Counts with CMB-cluster-lensing Data: Results from the SPT-SZ Survey and Forecasts for the Future","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"Argonne National Laboratory; Istituto Nazionale di Fisica Nucleare; Australian Research Council; Ministero dell’Istruzione, dell’Università e della Ricerca; High Energy Physics; U.S. Department of Energy; National Science Foundation","keywords":"Cosmic microwave background; Physics; Planck; Astrophysics; Galaxy cluster; South Pole Telescope; Dark energy; Cluster (spacecraft); Gravitational lens; Weak gravitational lensing; Galaxy; Sigma; Cosmology; Astronomy; Redshift","score_opus":0.019513985025690555,"score_gpt":0.23146959643902604,"score_spread":0.2119556114133355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214217376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9386415,0.0033503706,0.015651304,0.006539357,0.000157815,0.000026654097,0.020776406,0.0006247576,0.014231913],"genre_scores_gemma":[0.9794254,0.0006640069,0.006538013,0.0001647091,0.00012549997,0.000011585169,0.0117132785,0.00013009658,0.001227414],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992835,0.00018859004,0.000028354692,0.00017369454,0.0002711993,0.0000546747],"domain_scores_gemma":[0.99380624,0.0021709339,0.0010813924,0.00068693707,0.001602515,0.00065198925],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029058673,0.00065293786,0.00041643615,0.0012038001,0.00028114705,0.001726225,0.00071630545,0.00049371086,0.0028625056],"category_scores_gemma":[0.011641516,0.00033297198,0.0005231348,0.0016899607,0.0003469672,0.0023495795,0.00082329666,0.0008354205,0.000826562],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038640315,0.000060712715,0.885347,0.00014872568,0.00022740549,0.00012972506,0.00018452387,0.04431743,0.0021221268,0.0072456608,0.019415198,0.040415123],"study_design_scores_gemma":[0.000063352556,0.000048852085,0.8331415,0.000083365005,0.0001508762,0.000061471954,0.00031793132,0.13876732,0.0022622682,0.00895608,0.01605331,0.00009365625],"about_ca_topic_score_codex":0.058095936,"about_ca_topic_score_gemma":0.043164067,"teacher_disagreement_score":0.058095936,"about_ca_system_score_codex":0.0010668356,"about_ca_system_score_gemma":0.0008018749,"threshold_uncertainty_score":0.11551553},"labels":[],"label_agreement":null},{"id":"W3214242691","doi":"10.3847/1538-4357/ac5f03","title":"Bridging the Gap: Categorizing Gravitational-wave Events at the Transition between Neutron Stars and Black Holes","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"National Aeronautics and Space Administration","keywords":"Physics; Neutron star; LIGO; Astrophysics; Gravitational wave; Binary black hole; Black hole (networking); Population; Compact star; Context (archaeology); Astronomy","score_opus":0.030891793832796405,"score_gpt":0.3163287430043633,"score_spread":0.2854369491715669,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214242691","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998147,0.00012488238,0.00066309905,0.00004709802,0.0000043615596,0.000008252903,0.00020003709,0.000016129656,0.000789164],"genre_scores_gemma":[0.99898976,0.000025279136,0.00045308346,0.000014323443,0.000006117621,0.0000041719823,0.00038833436,0.0000078165385,0.000111265974],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9993819,0.00014146071,0.00006216188,0.00012778508,0.00015076417,0.0001359058],"domain_scores_gemma":[0.9948578,0.0024270471,0.0013426633,0.00033190174,0.00038980015,0.0006508542],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016979292,0.00021034105,0.00030202518,0.00539534,0.00038477927,0.0013637475,0.00041588966,0.0005233457,0.0020604508],"category_scores_gemma":[0.0075163627,0.000083659026,0.00028508028,0.001883158,0.000573278,0.001573241,0.001646291,0.00031626408,0.0004534768],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026157327,0.000035698366,0.9865514,0.000017394592,0.000028543198,0.00007614263,0.00068888406,0.0002733318,0.0014433467,0.000497437,0.00020466784,0.009921548],"study_design_scores_gemma":[0.000007885999,0.000046643556,0.99311924,0.000019214393,0.000015772308,0.00013851486,0.0016216337,0.0028651936,0.0006413015,0.00086935656,0.0006474251,0.000007861295],"about_ca_topic_score_codex":0.0024266313,"about_ca_topic_score_gemma":0.0023951752,"teacher_disagreement_score":0.00539534,"about_ca_system_score_codex":0.00025799067,"about_ca_system_score_gemma":0.00020289079,"threshold_uncertainty_score":0.008979619},"labels":[],"label_agreement":null},{"id":"W3214261856","doi":"10.3847/1538-4357/ac2954","title":"Identifying Circumgalactic Medium Absorption in QSO Spectra: A Bayesian Approach","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Princeton University","keywords":"Physics; Astrophysics; Galaxy; Redshift; Luminosity; Astronomy; Quasar; Sky; RADIUS","score_opus":0.01195884761628642,"score_gpt":0.22762719010149265,"score_spread":0.21566834248520622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214261856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7450447,0.000409029,0.24959232,0.0004251766,0.000008537608,0.00014747324,0.00071417977,0.00022332215,0.0034352988],"genre_scores_gemma":[0.9501121,0.00009978038,0.048252508,0.00007416406,0.000024190162,0.00005991012,0.0007142835,0.000034241268,0.00062881026],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99661726,0.002083604,0.00013988069,0.00047540682,0.0005265948,0.00015735535],"domain_scores_gemma":[0.9795284,0.016270332,0.0016652766,0.0010538325,0.0010701681,0.00041198914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.008412258,0.0004747486,0.00058014254,0.0030419033,0.0009877195,0.0021077783,0.0014539909,0.000949318,0.0026559227],"category_scores_gemma":[0.03892279,0.0005349625,0.0008598222,0.0013930777,0.000830868,0.0016663928,0.0013349615,0.00079761376,0.0005482553],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009227161,0.00054264924,0.68742263,0.0001453426,0.000661948,0.00046032266,0.0012297403,0.124838434,0.0060233097,0.019467436,0.0019203573,0.15636514],"study_design_scores_gemma":[0.0000708451,0.0001337419,0.116754994,0.00007750122,0.00018901649,0.00046321834,0.0005474028,0.8503538,0.0012009551,0.02875355,0.0013817134,0.00007334464],"about_ca_topic_score_codex":0.011693682,"about_ca_topic_score_gemma":0.011758306,"teacher_disagreement_score":0.011693682,"about_ca_system_score_codex":0.0008548859,"about_ca_system_score_gemma":0.0009720498,"threshold_uncertainty_score":0.044488788},"labels":[],"label_agreement":null},{"id":"W3214335030","doi":"10.3847/1538-4357/ac63cc","title":"COMAP Early Science. I. Overview","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Jet Propulsion Laboratory; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Toronto; Keck Institute for Space Studies; Agencia Nacional de Investigación y Desarrollo; Norges Forskningsråd; California Institute of Technology; University of Miami; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astronomy; Astrophysics; Astrobiology","score_opus":0.013630458946361152,"score_gpt":0.2406427020099085,"score_spread":0.22701224306354736,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214335030","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0006936332,0.016349599,0.013240261,0.02572654,0.0080206515,0.00034856354,0.039035182,0.034719925,0.86186564],"genre_scores_gemma":[0.013033928,0.047613837,0.026613992,0.015764799,0.012916966,0.0012153516,0.07994213,0.02646322,0.7764359],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99838305,0.00021072285,0.00009343176,0.0002536432,0.00077074446,0.00028837967],"domain_scores_gemma":[0.9950394,0.00035659765,0.00022395942,0.0010070492,0.0013759969,0.0019970806],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.0029864132,0.0015310905,0.0009008461,0.008111923,0.0022923846,0.00910262,0.0028872972,0.0024250215,0.396965],"category_scores_gemma":[0.0058749965,0.0010118006,0.0008048981,0.011385182,0.0012482789,0.006520259,0.007872828,0.003264826,0.41148984],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004549594,0.000019247189,0.00018041625,0.00040628167,0.000006360865,0.000034291803,0.000039750405,0.00008217457,0.00018285884,0.009294783,0.82740146,0.16230683],"study_design_scores_gemma":[0.0000019608603,0.0000025348688,0.00022693985,0.00006307821,9.384635e-7,0.000015853542,0.0000062154927,0.000013737039,0.00004987932,0.0014914587,0.9981238,0.0000036339457],"about_ca_topic_score_codex":0.0043960265,"about_ca_topic_score_gemma":0.0036637764,"teacher_disagreement_score":0.396965,"about_ca_system_score_codex":0.0031880052,"about_ca_system_score_gemma":0.0053253607,"threshold_uncertainty_score":0.86015624},"labels":[],"label_agreement":null},{"id":"W3214500067","doi":"10.3847/1538-4357/ac1a72","title":"Tidal Response and Shape of Hot Jupiters","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Hot Jupiter; Planet; Astrophysics; Exoplanet; Gas giant; Light curve; Astronomy","score_opus":0.010826070298307906,"score_gpt":0.22652635123913575,"score_spread":0.21570028094082785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214500067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99928766,0.000014647105,0.00019082915,0.0000101783835,8.3746147e-7,0.0000014731276,0.000039402097,0.000022504315,0.0004323842],"genre_scores_gemma":[0.99970704,0.000005711696,0.000051364204,0.0000036759748,7.726926e-7,9.47429e-7,0.000068355395,0.000005484405,0.00015662725],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999486,0.000007411837,0.000002332467,0.000018572626,0.000010671935,0.0000122269075],"domain_scores_gemma":[0.99972373,0.00006266404,0.000074100535,0.00004774026,0.0000400624,0.000051680705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001148351,0.00014230899,0.00016881783,0.00033475153,0.00024670493,0.0003157474,0.0002571839,0.0002655795,0.00093605893],"category_scores_gemma":[0.00092019915,0.00013944208,0.00021483898,0.00018755888,0.00026586402,0.00022339293,0.00029163604,0.000182539,0.00018727529],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081663235,0.00007440921,0.59009683,0.0000703137,0.00016905193,0.0009053432,0.0010539771,0.111938834,0.28029394,0.0015635723,0.0010350137,0.01198212],"study_design_scores_gemma":[0.000030319281,0.00033060016,0.8019378,0.000010449622,0.00003914804,0.0004976807,0.00041728173,0.16973796,0.025034232,0.00072331564,0.0011924572,0.00004868759],"about_ca_topic_score_codex":0.00211454,"about_ca_topic_score_gemma":0.0014095798,"teacher_disagreement_score":0.00211454,"about_ca_system_score_codex":0.0002635613,"about_ca_system_score_gemma":0.000069560105,"threshold_uncertainty_score":0.004204452},"labels":[],"label_agreement":null},{"id":"W3214551887","doi":"10.3847/1538-4357/ac1f21","title":"Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy Size−Mass Relation at z &lt; 1","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":81,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Japan Society for the Promotion of Science","keywords":"Physics; Galaxy; Subaru Telescope; Astrophysics; Relation (database); Astronomy; Stellar mass; Star formation","score_opus":0.017807108755149292,"score_gpt":0.26544477828441326,"score_spread":0.24763766952926397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214551887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6781901,0.0010257683,0.06967911,0.0037447028,0.00033589927,0.00014488764,0.09476221,0.06329947,0.08881777],"genre_scores_gemma":[0.870335,0.0002129519,0.044525534,0.00077294064,0.00020101022,0.00024088903,0.06565935,0.007982574,0.010069819],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99964035,0.00011717724,0.000006670171,0.00009365243,0.00008390795,0.000058283364],"domain_scores_gemma":[0.9984862,0.00053785817,0.00019458118,0.00030402615,0.00026525976,0.00021199018],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016335127,0.0006342155,0.00055345846,0.0011817006,0.00036192976,0.0010453714,0.00076833286,0.0003944028,0.012076025],"category_scores_gemma":[0.002835183,0.0003682765,0.00055189704,0.0011364066,0.0002818247,0.0007265557,0.00074222067,0.00078882533,0.005123972],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022798935,0.0003049387,0.23956846,0.00039390373,0.00026712165,0.000519438,0.00064416666,0.042622823,0.019328281,0.028284928,0.5232538,0.14253229],"study_design_scores_gemma":[0.00037913816,0.00023276235,0.46402353,0.00011991354,0.00014560536,0.00037585848,0.0002515873,0.42555138,0.02481212,0.020504417,0.06348074,0.00012299966],"about_ca_topic_score_codex":0.0051595257,"about_ca_topic_score_gemma":0.0068517425,"teacher_disagreement_score":0.012076025,"about_ca_system_score_codex":0.00047582548,"about_ca_system_score_gemma":0.00034351557,"threshold_uncertainty_score":0.0403983},"labels":[],"label_agreement":null},{"id":"W3214565625","doi":"10.3847/1538-4357/ac8d04","title":"“Super-kilonovae” from Massive Collapsars as Signatures of Black Hole Birth in the Pair-instability Mass Gap","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"Natural Sciences and Engineering Research Council of Canada; Compute Canada; Simons Foundation; National Science Foundation","keywords":"Physics; Instability; Quantum mechanics","score_opus":0.012119266846826198,"score_gpt":0.23087197897234638,"score_spread":0.21875271212552017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214565625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989073,0.000112470494,0.00026216343,0.000017613303,0.0000033098208,0.0000028947838,0.000031671945,0.000013066274,0.00064950954],"genre_scores_gemma":[0.9995938,0.000030946536,0.00017866172,0.00001357652,0.00000470216,0.0000027727376,0.000056732482,0.000004157604,0.00011476266],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999502,0.0000053321282,0.0000026982868,0.000011052945,0.000013881771,0.000016856367],"domain_scores_gemma":[0.9997725,0.000039231105,0.000098144425,0.000024444787,0.000013502746,0.000052235933],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014987541,0.00017034035,0.00015057917,0.0005744121,0.00025799952,0.0003924851,0.0001871828,0.00028848072,0.0010308488],"category_scores_gemma":[0.0002826885,0.00012264265,0.00012658305,0.00018063858,0.0003110144,0.0001948512,0.0008384878,0.000319647,0.00019759286],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00249057,0.00012898173,0.50130916,0.00008700407,0.00010714366,0.028508691,0.001138105,0.00086230197,0.44659084,0.0017886928,0.00051134493,0.016477207],"study_design_scores_gemma":[0.000041491185,0.0004966955,0.9426234,0.000021357851,0.000032884454,0.016123714,0.0007007453,0.0019479846,0.034005642,0.001385386,0.0025993707,0.000021507307],"about_ca_topic_score_codex":0.00018218324,"about_ca_topic_score_gemma":0.00023763167,"teacher_disagreement_score":0.0010308488,"about_ca_system_score_codex":0.00011075366,"about_ca_system_score_gemma":0.00003618946,"threshold_uncertainty_score":0.0034486055},"labels":[],"label_agreement":null},{"id":"W3214570905","doi":"10.3847/1538-4357/ac63c6","title":"COMAP Early Science. II. Pathfinder Instrument","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"European Research Council; Jet Propulsion Laboratory; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; California Institute of Technology; European Commission; Science and Technology Facilities Council; University of Toronto; Keck Institute for Space Studies; Agencia Nacional de Investigación y Desarrollo; Norges Forskningsråd; University of Miami; National Aeronautics and Space Administration; National Science Foundation","keywords":"Pathfinder; Antenna (radio); Computer science; Redshift; Remote sensing; Optics; Environmental science; Systems engineering; Physics; Galaxy; Telecommunications; Engineering; Geology; Astronomy","score_opus":0.008551545896655025,"score_gpt":0.2059182656950964,"score_spread":0.19736671979844136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214570905","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04979489,0.0015263915,0.05930472,0.012537335,0.0012665387,0.0036075187,0.15146111,0.062202327,0.6582992],"genre_scores_gemma":[0.31181058,0.0023035142,0.2812873,0.00582535,0.00093155593,0.0031373773,0.14063835,0.008133944,0.24593198],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99903667,0.00009435983,0.000022943525,0.00015439889,0.0005311272,0.00016049923],"domain_scores_gemma":[0.99803525,0.00017703512,0.00010903833,0.00036886593,0.0009277756,0.00038206746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019697945,0.00062447414,0.00038604246,0.002992203,0.0018552787,0.0019088828,0.0016959494,0.0011194615,0.050059132],"category_scores_gemma":[0.0021778552,0.00043541158,0.0002811449,0.003423869,0.00071410014,0.0016401323,0.0022916791,0.0016483135,0.033217687],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00095638505,0.00017724477,0.015159301,0.00056206674,0.000031165164,0.00063063257,0.00038409577,0.0023093314,0.016264163,0.022607591,0.46286637,0.4780517],"study_design_scores_gemma":[0.00011095273,0.00013531094,0.016467607,0.00010643938,0.000009496016,0.00032278727,0.00010207486,0.0024751686,0.00881058,0.0045325365,0.9668846,0.000042320295],"about_ca_topic_score_codex":0.011082701,"about_ca_topic_score_gemma":0.010972025,"teacher_disagreement_score":0.050059132,"about_ca_system_score_codex":0.0027582978,"about_ca_system_score_gemma":0.0038872785,"threshold_uncertainty_score":0.1674645},"labels":[],"label_agreement":null},{"id":"W3214616473","doi":"10.3847/1538-4357/ac63c8","title":"COMAP Early Science. VI. A First Look at the COMAP Galactic Plane Survey","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Jet Propulsion Laboratory; Universitetet i Oslo; University of Toronto; Keck Institute for Space Studies; Norges Forskningsråd; California Institute of Technology; University of Miami; European Research Council; National Science Foundation","keywords":"Galactic plane; Physics; Astrophysics; Astronomy; Galaxy","score_opus":0.014511183001523476,"score_gpt":0.22996551675612775,"score_spread":0.21545433375460427,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214616473","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.17874004,0.0057324646,0.0047341594,0.01761139,0.0012657763,0.0003487153,0.58862364,0.0052346974,0.1977091],"genre_scores_gemma":[0.4536079,0.0048965053,0.018140756,0.004358283,0.00092307566,0.00032743576,0.42917803,0.0018301134,0.08673787],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9995364,0.000052074945,0.00001135681,0.00005941839,0.00020066122,0.00014013528],"domain_scores_gemma":[0.9978313,0.000102238664,0.00025553512,0.00029154573,0.000776643,0.0007427308],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007923636,0.00049816084,0.00020328815,0.0038623947,0.0008544592,0.0016360842,0.00050155685,0.00041167595,0.017503029],"category_scores_gemma":[0.0017438625,0.00022899566,0.00015598162,0.0063463445,0.0002417958,0.00072235055,0.0013817949,0.0006502945,0.010046662],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002992463,0.00008051855,0.12533042,0.000313284,0.000066233,0.00048896176,0.0003657345,0.00043207034,0.002118164,0.0035562909,0.6904598,0.17648922],"study_design_scores_gemma":[0.000022134354,0.000037347607,0.4153647,0.00008173985,0.000008257715,0.00016672941,0.00025827976,0.00036225189,0.0006590988,0.0007740048,0.582248,0.000017455646],"about_ca_topic_score_codex":0.062129334,"about_ca_topic_score_gemma":0.06786922,"teacher_disagreement_score":0.062129334,"about_ca_system_score_codex":0.0012818396,"about_ca_system_score_gemma":0.0015700184,"threshold_uncertainty_score":0.123535395},"labels":[],"label_agreement":null},{"id":"W3214723061","doi":"10.3847/1538-4357/ac7a37","title":"SNIa Cosmology Analysis Results from Simulated LSST Images: From Difference Imaging to Constraints on Dark Energy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of New Brunswick","funders":"Science and Technology Facilities Council; Centre National de la Recherche Scientifique; Institut National de Physique Nucléaire et de Physique des Particules; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Dark energy; Photometry (optics); Astrophysics; Observatory; Large Synoptic Survey Telescope; Supernova; Cosmology; Magnitude (astronomy); Astronomy; Galaxy; Stars","score_opus":0.009447769998490405,"score_gpt":0.2293236761873065,"score_spread":0.2198759061888161,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214723061","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9882939,0.00009459909,0.00781492,0.00019548165,0.000015178047,0.000024647494,0.00094774185,0.00071254995,0.0019009389],"genre_scores_gemma":[0.98900175,0.00002712023,0.007857325,0.000063337335,0.000008985141,0.00001671036,0.0026656848,0.00014953557,0.00020967175],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995171,0.00015047773,0.000029506578,0.00014481352,0.00009276873,0.00006529449],"domain_scores_gemma":[0.9964311,0.0017428793,0.0002779871,0.00062869437,0.00060547504,0.00031394468],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017964066,0.00054718193,0.00049042335,0.0006438964,0.00043519394,0.0010357858,0.0012325858,0.0005781342,0.0016372919],"category_scores_gemma":[0.007053118,0.00039951308,0.0010588161,0.0007023528,0.00055608014,0.0006460684,0.00090331247,0.0008420837,0.00022944632],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006683718,0.0001573545,0.10982902,0.00006530481,0.0003981169,0.00016274647,0.0001408214,0.87115747,0.004417426,0.003001823,0.0018144681,0.008187009],"study_design_scores_gemma":[0.00008107359,0.00006198717,0.020061415,0.000008082628,0.000029532841,0.000053017102,0.00005266827,0.9762841,0.0018716686,0.0009916341,0.00048619483,0.000018619736],"about_ca_topic_score_codex":0.032184117,"about_ca_topic_score_gemma":0.018028146,"teacher_disagreement_score":0.032184117,"about_ca_system_score_codex":0.0014537417,"about_ca_system_score_gemma":0.00087408995,"threshold_uncertainty_score":0.06399357},"labels":[],"label_agreement":null},{"id":"W3214963737","doi":"10.3847/1538-4357/ac341c","title":"Diagnosing DASH: A Catalog of Structural Properties for the COSMOS-DASH Survey","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; York University; University of Toronto","funders":"Danmarks Grundforskningsfond; National Aeronautics and Space Administration; California Institute of Technology; Nuclear Safety and Security Commission; National Research Foundation; Alfred P. Sloan Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Galaxy; Algorithm; Astrophysics; Computer science","score_opus":0.02117273399294732,"score_gpt":0.23085217495250218,"score_spread":0.20967944095955487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3214963737","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.50018805,0.0007887134,0.006943376,0.00017347814,0.000069139125,0.00034728402,0.45617926,0.004894079,0.030416653],"genre_scores_gemma":[0.25508967,0.0005956094,0.010845411,0.00016744215,0.00010407542,0.00056134874,0.72280204,0.0009279593,0.008906391],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99944335,0.0000653005,0.00007047899,0.00015439017,0.0001987831,0.00006769636],"domain_scores_gemma":[0.9969554,0.00021497114,0.00066190393,0.00082747615,0.0006641663,0.0006761604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009933175,0.0007014879,0.0004574452,0.005686538,0.00035664698,0.0010409942,0.0006941172,0.00020196318,0.014767914],"category_scores_gemma":[0.00213338,0.0002861979,0.0003206371,0.0051172073,0.00019015968,0.00081028155,0.0016167184,0.00033126253,0.010851651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036529824,0.00016474533,0.76759833,0.00028771305,0.00016238868,0.00022844852,0.0003827263,0.0012613954,0.009915868,0.0019095554,0.12447277,0.09325067],"study_design_scores_gemma":[0.00009395477,0.000087777735,0.7889273,0.000055051885,0.000051087045,0.00031349543,0.00034920234,0.0019360264,0.0030434104,0.0011261747,0.20397381,0.00004270856],"about_ca_topic_score_codex":0.0034289896,"about_ca_topic_score_gemma":0.0037802574,"teacher_disagreement_score":0.014767914,"about_ca_system_score_codex":0.00027645743,"about_ca_system_score_gemma":0.00044389305,"threshold_uncertainty_score":0.049403608},"labels":[],"label_agreement":null},{"id":"W3215932904","doi":"10.3847/1538-4357/ac3bba","title":"Light-curve Evolution of the Nearest Tidal Disruption Event: A Late-time, Radio-only Flare","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Associated Universities; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Flare; Astrophysics; Supermassive black hole; Astronomy; Jansky; Galaxy; Light curve; Accretion (finance); Flux (metallurgy); Radio galaxy","score_opus":0.006246253007449214,"score_gpt":0.21138939328851222,"score_spread":0.205143140281063,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3215932904","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964366,0.000054176133,0.00018883162,0.0000599467,0.0000093118915,0.000010346837,0.0010528415,0.000043934593,0.0021441018],"genre_scores_gemma":[0.9981895,0.000014352222,0.00013733064,0.00001936339,0.000008054253,0.0000029940495,0.001172395,0.0000049080663,0.00045098842],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999182,0.000005332588,0.000004848371,0.000024391758,0.000016594282,0.000030594816],"domain_scores_gemma":[0.9990594,0.00010340573,0.00021498847,0.00004716436,0.0002232991,0.0003517956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019695747,0.00018443586,0.00019111998,0.0011648262,0.00022755828,0.0004992099,0.00024202459,0.00048012764,0.0013351471],"category_scores_gemma":[0.00067335606,0.00008344836,0.00021208686,0.0004990677,0.00014244924,0.00023965168,0.00025742187,0.0003384344,0.00046587098],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002152886,0.00015664507,0.975195,0.000019207084,0.000049157516,0.00035835098,0.00020778121,0.0015727398,0.010868501,0.00019253785,0.001623106,0.009541752],"study_design_scores_gemma":[0.0000022345107,0.0000405114,0.9971885,0.0000028818847,0.000007296458,0.00008030189,0.000056493784,0.0018578318,0.00031147682,0.000023447852,0.00042492425,0.000004099568],"about_ca_topic_score_codex":0.017518615,"about_ca_topic_score_gemma":0.025614088,"teacher_disagreement_score":0.017518615,"about_ca_system_score_codex":0.00055429415,"about_ca_system_score_gemma":0.00012084699,"threshold_uncertainty_score":0.034833252},"labels":[],"label_agreement":null},{"id":"W3215962913","doi":"10.3847/1538-4357/ac236c","title":"Constraining Progenitors of Observed Low-mass X-ray Binaries Using Convection and Rotation-Boosted Magnetic Braking","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Astrophysics; Physics; Low Mass; Population; Mass transfer; Rotation (mathematics); Binary number; Stellar mass; Astronomy; Stars; Star formation; Mechanics","score_opus":0.02569598021535836,"score_gpt":0.23890678392045137,"score_spread":0.21321080370509302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3215962913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92382133,0.00021323003,0.07237637,0.00004906887,0.00001730308,0.00003204882,0.00054976996,0.00072149094,0.0022194618],"genre_scores_gemma":[0.95905757,0.000048937443,0.039934486,0.000019046838,0.000008297317,0.000026262162,0.00056078495,0.00008521723,0.00025932927],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99988914,0.000031503256,0.0000071683226,0.00003489328,0.000025656138,0.000011720444],"domain_scores_gemma":[0.9993358,0.00022053665,0.00014356861,0.00018079036,0.000059418533,0.000059841346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006053059,0.0002547486,0.00024811982,0.00053081935,0.00028596772,0.0005425683,0.00047598768,0.00023622678,0.00086514885],"category_scores_gemma":[0.0018476817,0.00026814902,0.0003368391,0.00022373484,0.00020837225,0.00027771993,0.0006449036,0.00034454593,0.00027203918],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000500735,0.00012833046,0.36070788,0.00013565159,0.00030309483,0.00022224114,0.00023435295,0.38577506,0.15898591,0.007936938,0.0007768838,0.084292896],"study_design_scores_gemma":[0.000066155575,0.000096639444,0.038634125,0.000013773081,0.000050205163,0.00012461355,0.000029254097,0.91313344,0.043221954,0.0021724994,0.002428832,0.00002862263],"about_ca_topic_score_codex":0.0019924717,"about_ca_topic_score_gemma":0.0024165164,"teacher_disagreement_score":0.0019924717,"about_ca_system_score_codex":0.00037039418,"about_ca_system_score_gemma":0.00034014467,"threshold_uncertainty_score":0.003961742},"labels":[],"label_agreement":null},{"id":"W3216138489","doi":"10.3847/1538-4357/ac4d29","title":"Improved Characterization of the Astrophysical Muon–neutrino Flux with 9.5 Years of IceCube Data","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":234,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Santen; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; University of Oxford; Compute Canada; Marquette University; University of Wisconsin-Madison; U.S. Department of Energy; Vetenskapsrådet","keywords":"Physics; Algorithm; Computer science","score_opus":0.00960864209081109,"score_gpt":0.20874630286665313,"score_spread":0.19913766077584205,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3216138489","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88381284,0.001341162,0.03344715,0.00038691584,0.00014941367,0.00014060298,0.060898922,0.0010360025,0.018787038],"genre_scores_gemma":[0.8995684,0.00038151754,0.024181139,0.00013743252,0.0001084718,0.00020464424,0.07380889,0.0002919937,0.001317472],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987815,0.00033645023,0.000089748515,0.00038278967,0.0002689808,0.00014047218],"domain_scores_gemma":[0.9970452,0.0007190057,0.00060715363,0.00079659035,0.0006680142,0.0001641371],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0033080191,0.0006410088,0.00064835843,0.0016483323,0.00044540412,0.0014032552,0.00063249876,0.00051678135,0.0020488824],"category_scores_gemma":[0.0037155997,0.00030826573,0.00079918146,0.0019719107,0.00025017196,0.0010555136,0.0007798381,0.00056934945,0.00079493603],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031567137,0.00051248434,0.7635814,0.00044538136,0.0012194287,0.00074911834,0.000447812,0.06424685,0.06573336,0.008969642,0.013767677,0.07717011],"study_design_scores_gemma":[0.00018164792,0.00022500669,0.79252726,0.00015246101,0.0002644149,0.0005281869,0.00010307139,0.06328715,0.064015284,0.0029911997,0.07557851,0.00014573411],"about_ca_topic_score_codex":0.0062440513,"about_ca_topic_score_gemma":0.007015565,"teacher_disagreement_score":0.0062440513,"about_ca_system_score_codex":0.0009254634,"about_ca_system_score_gemma":0.0004911103,"threshold_uncertainty_score":0.017494678},"labels":[],"label_agreement":null},{"id":"W3216175927","doi":"10.3847/1538-4357/ac404a","title":"SQuIGGLE : Studying Quenching in Intermediate-z Galaxies—Gas, AnguLar Momentum, and Evolution","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of California, Los Angeles; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; Jet Propulsion Laboratory; Princeton University; Aspen Center for Physics; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Alfred P. Sloan Foundation; University of Washington; National Science Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Redshift; Luminous infrared galaxy; Star formation; Stellar mass; Sky; Astronomy; Galaxy formation and evolution; Quenching (fluorescence)","score_opus":0.013951224180304004,"score_gpt":0.27352373907652894,"score_spread":0.25957251489622496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3216175927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8064817,0.0014092928,0.11389992,0.0009191018,0.00008646254,0.00022227634,0.011185026,0.028453784,0.037342552],"genre_scores_gemma":[0.9420423,0.00016119215,0.042145964,0.00042049948,0.000049281516,0.00011947477,0.0049123624,0.0023887379,0.007760179],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999828,0.000027548362,0.0000041592994,0.000050769657,0.000048307305,0.000041256702],"domain_scores_gemma":[0.9992712,0.00015466094,0.00008084969,0.00020193221,0.00008044836,0.0002109574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087866216,0.00041711432,0.0004317488,0.0006336119,0.00047584975,0.0007539626,0.00092191214,0.00032483359,0.007212703],"category_scores_gemma":[0.0009937311,0.00029202498,0.0006418659,0.0005234595,0.00033089766,0.0008146049,0.0011500437,0.0009393512,0.0017695095],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014640822,0.0005995287,0.36784026,0.0005656878,0.000672256,0.0006845319,0.0025855282,0.039556816,0.2100721,0.023472734,0.06492513,0.2875613],"study_design_scores_gemma":[0.00023798671,0.00058600394,0.63848716,0.00007331692,0.00019596089,0.00055141764,0.0006490157,0.19319692,0.08514683,0.029366432,0.05130201,0.00020691636],"about_ca_topic_score_codex":0.008903529,"about_ca_topic_score_gemma":0.010177561,"teacher_disagreement_score":0.008903529,"about_ca_system_score_codex":0.0007957386,"about_ca_system_score_gemma":0.00030874225,"threshold_uncertainty_score":0.024128854},"labels":[],"label_agreement":null},{"id":"W3216299966","doi":"10.3847/1538-4357/ac74bb","title":"Constraints on the Cosmic Expansion History from GWTC–3","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":229,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; University of British Columbia; Perimeter Institute","funders":"European Social Fund; Great Southern Development Commission, Government of Western Australia; Japan Society for the Promotion of Science; Science and Technology Facilities Council; ICTP South American Institute for Fundamental Research; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, India; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat Valenciana; Istituto Nazionale di Fisica Nucleare; Generalitat de Catalunya; U.S. Department of Energy; National Natural Science Foundation of China; National Research, Development and Innovation Office; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Korea Institute of Science and Technology Information; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Institute for Cosmic Ray Research, University of Tokyo; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; Ministerio de Ciencia e Innovación; European Commission; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Institut des Origines de Lyon; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; European Regional Development Fund; Scottish Universities Physics Alliance; Centres de Recerca de Catalunya; Fonds Wetenschappelijk Onderzoek; Division of Human Resource Development; University of Pennsylvania; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; Redshift; Astrophysics; LIGO; Galaxy; Hubble's law; Luminosity; Population; Mass distribution; Gravitational wave; Astronomy","score_opus":0.027408844748798098,"score_gpt":0.30138226668615464,"score_spread":0.2739734219373565,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3216299966","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97656417,0.0001957345,0.0038206796,0.00011411398,0.000011801957,0.000020168436,0.011906309,0.00036573282,0.007001294],"genre_scores_gemma":[0.9789934,0.00006704444,0.001328219,0.000031643467,0.0000242478,0.000018195957,0.019026503,0.00007054611,0.0004401455],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997695,0.000024804101,0.000016817197,0.000051014933,0.00008064367,0.000057203037],"domain_scores_gemma":[0.996563,0.0007035115,0.001185035,0.0007209019,0.0004636881,0.00036392035],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006872945,0.00025474833,0.00025011212,0.0022401891,0.00028448648,0.0009452488,0.00031830376,0.0002844157,0.0031411215],"category_scores_gemma":[0.0034959603,0.00016115887,0.00033011872,0.002216105,0.00021076146,0.00043058625,0.0006062424,0.00029689932,0.00088297273],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028268225,0.000041739833,0.95833826,0.00003716881,0.000081141894,0.00014960444,0.00016941609,0.0032643366,0.006682406,0.00339236,0.0034593476,0.024101458],"study_design_scores_gemma":[0.000013038973,0.000013895383,0.98626167,0.000014197296,0.000022908978,0.00008612874,0.000025925927,0.007333248,0.0015196161,0.0007975123,0.0039006746,0.000011090417],"about_ca_topic_score_codex":0.010006062,"about_ca_topic_score_gemma":0.0117408205,"teacher_disagreement_score":0.010006062,"about_ca_system_score_codex":0.00054744305,"about_ca_system_score_gemma":0.00040309707,"threshold_uncertainty_score":0.019895673},"labels":[],"label_agreement":null},{"id":"W3216924585","doi":"10.3847/1538-4357/ac222f","title":"The Viscosity Parameter for Late-type Stable Be Stars","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Stars; Angular momentum; Viscosity; Star (game theory); Isothermal process; Specific relative angular momentum; Classical mechanics; Total angular momentum quantum number; Thermodynamics; Angular momentum coupling","score_opus":0.018680664967431995,"score_gpt":0.2600117547060291,"score_spread":0.24133108973859713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3216924585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99667406,0.00012813765,0.0021881808,0.000023852992,0.0000023559285,0.0000046509904,0.00004632445,0.00001730929,0.00091503776],"genre_scores_gemma":[0.9996958,0.000021893837,0.0001967471,0.000002292441,0.0000011872561,0.0000013972083,0.000027987826,0.0000022630013,0.000050398703],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999589,0.0000055343244,0.0000031803631,0.000013205441,0.000008020382,0.000011239476],"domain_scores_gemma":[0.9995472,0.00014626472,0.00016547242,0.000021863461,0.00004208063,0.00007714918],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020969566,0.00023000354,0.00019489061,0.0007314135,0.00021411445,0.0006219664,0.00025036215,0.00034601256,0.00039160348],"category_scores_gemma":[0.0012025824,0.00014063009,0.0002103176,0.00028684316,0.00032674806,0.00038802563,0.0002990071,0.00022269327,0.00012355682],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007182879,0.00014737922,0.584885,0.00014215583,0.00012802148,0.0010875756,0.0006503787,0.19408552,0.18275093,0.017079597,0.00054471893,0.01778043],"study_design_scores_gemma":[0.000097066375,0.00030468128,0.3330608,0.000038149337,0.000046075864,0.0007339574,0.0003486971,0.6217144,0.033752147,0.008463358,0.0013787173,0.000061873616],"about_ca_topic_score_codex":0.0008870364,"about_ca_topic_score_gemma":0.0004969076,"teacher_disagreement_score":0.0008870364,"about_ca_system_score_codex":0.00034883813,"about_ca_system_score_gemma":0.00010479091,"threshold_uncertainty_score":0.002530992},"labels":[],"label_agreement":null},{"id":"W3217047019","doi":"10.3847/1538-4357/ac3dfa","title":"Now You See It, Now You Don’t: Star Formation Truncation Precedes the Loss of Molecular Gas by ∼100 Myr in Massive Poststarburst Galaxies at z ∼ 0.6","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Phase Equilibria and Thermodynamics","field":"Engineering","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Brookhaven National Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; National Institutes of Natural Sciences; Science and Technology Facilities Council; Jet Propulsion Laboratory; Office of Science; University of Illinois at Urbana-Champaign; Chinese Academy of Sciences; High Energy Physics; Deutsche Forschungsgemeinschaft; University of Sussex; York University; National Energy Research Scientific Computing Center; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; National Aeronautics and Space Administration; University College London; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Vanderbilt University; University of Chicago; U.S. Department of Energy; National Radio Astronomy Observatory; SLAC National Accelerator Laboratory; Harvard University; Ohio State University; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; Financiadora de Estudos e Projetos; University of Pennsylvania; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Yale University; Fermilab; National Science Foundation; California Institute of Technology; Aspen Center for Physics","keywords":"Physics; Astrophysics; Galaxy; Star formation; Stellar mass; Sky; Star (game theory); Galaxy formation and evolution; Population; Astronomy; Stellar population","score_opus":0.00642591510321433,"score_gpt":0.21626194818542416,"score_spread":0.20983603308220983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3217047019","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99691474,0.00008428724,0.00039139754,0.00020944438,0.000012214236,0.000003257246,0.00056950696,0.00008222479,0.00173279],"genre_scores_gemma":[0.9976761,0.00003320321,0.00024270278,0.00008040086,0.0000071819027,0.0000029803025,0.0006492128,0.00001237551,0.0012960298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994934,0.0000032780158,0.0000018004646,0.000019016397,0.000011205731,0.000015418302],"domain_scores_gemma":[0.99967265,0.000036845926,0.00007816733,0.00004464761,0.00005692736,0.000110685636],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019467999,0.000056925226,0.00011283212,0.00015347588,0.00018956298,0.00031195546,0.00015569958,0.00016912508,0.0036735998],"category_scores_gemma":[0.0006604046,0.000065089094,0.00013261383,0.0001280127,0.00015215311,0.00032950495,0.00023727553,0.00028807286,0.0008859437],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005763291,0.00008641545,0.9169939,0.000031557516,0.000032141408,0.0001651724,0.0005115432,0.0006868552,0.046918422,0.00081756955,0.0040141605,0.029165976],"study_design_scores_gemma":[0.000004888418,0.00007815451,0.9932695,0.0000047088765,0.0000053070307,0.000060445676,0.000102941645,0.0003813523,0.0041204654,0.0001621773,0.0018068521,0.0000032792848],"about_ca_topic_score_codex":0.0053402944,"about_ca_topic_score_gemma":0.0073951026,"teacher_disagreement_score":0.0053402944,"about_ca_system_score_codex":0.00021376523,"about_ca_system_score_gemma":0.00010240272,"threshold_uncertainty_score":0.0122894645},"labels":[],"label_agreement":null},{"id":"W3217198862","doi":"10.3847/1538-4357/ac3af4","title":"K-band Imaging of the Nearby Clumpy, Turbulent Disk Galaxy DYNAMO G04-1","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Dynamo; Galaxy; Stellar mass; Star (game theory); Star formation; Astronomy; Magnetic field","score_opus":0.004590695391622362,"score_gpt":0.1979559947530146,"score_spread":0.19336529936139224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3217198862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998638,0.000037724025,0.00038785845,0.000016236745,0.0000018821027,0.0000042815527,0.00018395703,0.000049640246,0.0006804554],"genre_scores_gemma":[0.99690574,0.000032907454,0.0021785263,0.000023874652,0.000005216258,0.0000038995454,0.00043712652,0.00001957766,0.000393073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992883,0.000005320595,0.0000038044236,0.00002083433,0.000014434353,0.000026811575],"domain_scores_gemma":[0.99981886,0.000019033636,0.00004896965,0.00002491809,0.000030321886,0.00005792436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013064766,0.00014893276,0.0001326581,0.0016036646,0.00033303452,0.00034475033,0.00030961563,0.0002754823,0.0008105526],"category_scores_gemma":[0.00021687197,0.00012858943,0.00015814025,0.00054059096,0.00015773303,0.00015289454,0.00044289097,0.00013939888,0.00032793081],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000555161,0.0001543153,0.63540816,0.0000819743,0.00009935999,0.0032786843,0.0009961241,0.002766803,0.32619935,0.0003667111,0.00166251,0.02843078],"study_design_scores_gemma":[0.000011518482,0.00008673749,0.9816451,0.0000087330745,0.000028113038,0.0016217143,0.0003054727,0.00418796,0.010728189,0.000114067465,0.0012518981,0.000010535043],"about_ca_topic_score_codex":0.0022173251,"about_ca_topic_score_gemma":0.004994582,"teacher_disagreement_score":0.0022173251,"about_ca_system_score_codex":0.00020035647,"about_ca_system_score_gemma":0.00008062831,"threshold_uncertainty_score":0.004408896},"labels":[],"label_agreement":null},{"id":"W3217208672","doi":"10.3847/1538-4357/ac8675","title":"Gravitational Wave Sources in Our Galactic Backyard: Predictions for BHBH, BHNS, and NSNS Binaries Detectable with LISA","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"European Research Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Foundation","keywords":"Physics; Gravitational wave; Astrophysics; Neutron star; Milky Way; Astronomy; Pulsar; Population; Metallicity; Supernova; White dwarf; Black hole (networking); Stars","score_opus":0.012667354928449722,"score_gpt":0.28335894376855436,"score_spread":0.27069158884010464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3217208672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99336374,0.00007285007,0.0033084673,0.00032119607,0.0000056356234,0.000013967044,0.00043225734,0.0000736622,0.0024081436],"genre_scores_gemma":[0.9985238,0.000027272614,0.0007699861,0.000047585698,0.000006775179,0.000008569654,0.00030017665,0.000015348909,0.0003006075],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998573,0.00003446442,0.0000072128178,0.000044939363,0.000025647274,0.00003035812],"domain_scores_gemma":[0.99867696,0.00059949735,0.00020806945,0.000087269276,0.00014725573,0.00028088322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009208355,0.00037013015,0.00044794244,0.0006861129,0.0005731597,0.0013253954,0.00088074896,0.0006281416,0.0018635439],"category_scores_gemma":[0.0028390249,0.00041012655,0.0006490886,0.00032341704,0.00057827967,0.0010007895,0.0006316003,0.00039923098,0.00054914696],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024976482,0.000098037446,0.56809527,0.00003149397,0.00009825394,0.0002550996,0.00019059172,0.41046488,0.0036762208,0.010145715,0.0010136537,0.0056811008],"study_design_scores_gemma":[0.00006810332,0.00009271401,0.12964642,0.000020975629,0.000036238176,0.00007545126,0.00015336084,0.8621771,0.0013247553,0.00585371,0.00051636476,0.000034820114],"about_ca_topic_score_codex":0.010053973,"about_ca_topic_score_gemma":0.0072821146,"teacher_disagreement_score":0.010053973,"about_ca_system_score_codex":0.0013470255,"about_ca_system_score_gemma":0.00041742102,"threshold_uncertainty_score":0.019990861},"labels":[],"label_agreement":null},{"id":"W3217286902","doi":"10.3847/1538-4357/ac3ed6","title":"Kepler-167e as a Probe of the Formation Histories of Cold Giants with Inner Super-Earths","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Astronomy; Kepler; Astrobiology; Astrophysics; Planet","score_opus":0.00784364792812507,"score_gpt":0.1934612454360458,"score_spread":0.18561759750792073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3217286902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960937,0.0001404078,0.0004543778,0.00005405718,0.0000049236264,0.0000075324833,0.0007781358,0.00008204494,0.0023848678],"genre_scores_gemma":[0.9977277,0.000029963327,0.00082882826,0.000037349397,0.000004636535,0.000007011429,0.00077126245,0.000024705969,0.0005685736],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999095,0.000010284979,0.000004528039,0.000037176884,0.000016898332,0.000021537517],"domain_scores_gemma":[0.99933785,0.000113856055,0.0002228664,0.00009929651,0.00006820371,0.00015782719],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003108875,0.00012805739,0.00023788965,0.0007376819,0.00027685546,0.0004234548,0.00019741415,0.00029489218,0.001703907],"category_scores_gemma":[0.0007663118,0.00012151813,0.00012196274,0.00042632286,0.00022752707,0.00039672133,0.0005892408,0.00031837085,0.0006775054],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006831726,0.00009270617,0.8897257,0.00009752972,0.000082261984,0.00048439458,0.00084785896,0.0009283017,0.07939423,0.0015517517,0.0021101136,0.02400198],"study_design_scores_gemma":[0.000017629363,0.00015588252,0.97957695,0.000013637344,0.000021332058,0.0006449971,0.00026731263,0.0021219633,0.012321519,0.00032510032,0.0045169233,0.000016803104],"about_ca_topic_score_codex":0.001077382,"about_ca_topic_score_gemma":0.0022278386,"teacher_disagreement_score":0.001703907,"about_ca_system_score_codex":0.00023806412,"about_ca_system_score_gemma":0.00010478231,"threshold_uncertainty_score":0.005700171},"labels":[],"label_agreement":null},{"id":"W3217405118","doi":"10.3847/1538-4357/aca7be","title":"Applying the Metallicity-dependent Binary Fraction to Double White Dwarf Formation: Implications for LISA","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; White dwarf; Metallicity; Astrophysics; Binary number; Binary star; Astronomy; Blue dwarf; Stars","score_opus":0.03980449259313313,"score_gpt":0.36262073003334944,"score_spread":0.3228162374402163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3217405118","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967675,0.000053996846,0.0013877269,0.00012996554,0.0000062209792,0.000012540325,0.000308857,0.000054482352,0.0012787399],"genre_scores_gemma":[0.9987367,0.000026041625,0.0008701196,0.000025980105,0.0000029928751,0.0000079332085,0.00014698028,0.00001699591,0.00016631509],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998275,0.000065107735,0.00000847788,0.00004121645,0.00002238213,0.00003530396],"domain_scores_gemma":[0.9987488,0.0007009594,0.00017044917,0.00011352912,0.000119051605,0.00014717675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00088616915,0.00034596206,0.00044837457,0.0004595297,0.0006583306,0.0010718037,0.000754121,0.00069152965,0.0012427144],"category_scores_gemma":[0.0035264196,0.00022463665,0.0005200925,0.00038593076,0.0005926992,0.0005272959,0.00056981825,0.00045821373,0.00016077331],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021497684,0.00011410858,0.17429166,0.000043416687,0.000085464846,0.00023093428,0.00013025024,0.8147465,0.003115592,0.0032579864,0.00052071235,0.0032483377],"study_design_scores_gemma":[0.00007125239,0.0001438929,0.033603992,0.000017602932,0.00004403208,0.00010070195,0.00015643411,0.9612376,0.0021232825,0.0016986537,0.000781299,0.000021225294],"about_ca_topic_score_codex":0.016869444,"about_ca_topic_score_gemma":0.011647102,"teacher_disagreement_score":0.016869444,"about_ca_system_score_codex":0.0014123081,"about_ca_system_score_gemma":0.000647125,"threshold_uncertainty_score":0.033542514},"labels":[],"label_agreement":null},{"id":"W3217440745","doi":"10.3847/1538-4357/ac1c03","title":"3-OGC: Catalog of Gravitational Waves from Compact-binary Mergers","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":196,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Database; LIGO; Binary number; Algorithm; Gravitational wave; Astrophysics; Computer science; Mathematics","score_opus":0.014811610087942592,"score_gpt":0.31031836910005883,"score_spread":0.29550675901211626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W3217440745","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.23500697,0.0039262446,0.006616802,0.00048967276,0.00023271158,0.00090504676,0.709087,0.006166015,0.037569467],"genre_scores_gemma":[0.08934115,0.0012840667,0.007363266,0.00026093618,0.00018745141,0.00036771956,0.896498,0.00072878675,0.003968598],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988336,0.0000735541,0.00016004952,0.0001834312,0.0005106393,0.00023869083],"domain_scores_gemma":[0.9947825,0.00045765485,0.0014333973,0.0010512191,0.0014150018,0.00086022506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011085597,0.000949417,0.0006616779,0.016781956,0.0008337434,0.0022597408,0.0008574304,0.00054144545,0.008017423],"category_scores_gemma":[0.004628971,0.0002947969,0.00069128786,0.014370187,0.0003273645,0.0012067886,0.0021669774,0.0006742821,0.005968043],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006460324,0.00016235236,0.37966466,0.00090209127,0.00022385533,0.0006626652,0.000834907,0.0013391848,0.0056052925,0.0072539537,0.43851766,0.16418728],"study_design_scores_gemma":[0.0001478206,0.000059103455,0.5481431,0.00029670444,0.00014148427,0.00073911774,0.00043909793,0.0032554974,0.0032012272,0.0025541375,0.4409239,0.000098770426],"about_ca_topic_score_codex":0.026866358,"about_ca_topic_score_gemma":0.018459626,"teacher_disagreement_score":0.026866358,"about_ca_system_score_codex":0.0011264853,"about_ca_system_score_gemma":0.0024144298,"threshold_uncertainty_score":0.053419948},"labels":[],"label_agreement":null},{"id":"W4200007105","doi":"10.3847/1538-4357/ac26c3","title":"HST/WFC3 Grism Observations of z ∼ 1 Clusters: Evidence for Rapid Outside-in Environmental Quenching from Spatially Resolved Hα Maps","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Waterloo; York University","funders":"Astrophysics Division; Centro de Astrofísica y Tecnologías Afines; Space Telescope Science Institute; National Research Foundation; National Aeronautics and Space Administration; Danmarks Grundforskningsfond; National Science Foundation","keywords":"Grism; Physics; Quenching (fluorescence); Astrophysics; Astronomy; Galaxy; Redshift; Optics; Fluorescence","score_opus":0.029151337555903527,"score_gpt":0.2399453351222682,"score_spread":0.2107939975663647,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200007105","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98634076,0.00021584479,0.0021901776,0.00014979162,0.000013406486,0.000017698705,0.0049815825,0.00075754593,0.005333241],"genre_scores_gemma":[0.99348056,0.000065901804,0.0015036864,0.0000804462,0.000021533355,0.000009627125,0.0040549967,0.00017229025,0.0006108686],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997718,0.000016101507,0.0000077881405,0.00006662952,0.000081485276,0.000056181834],"domain_scores_gemma":[0.99927646,0.000053937456,0.00022531798,0.00016449422,0.00013611882,0.00014365568],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043958408,0.00022193062,0.00026006813,0.0009885851,0.00035554622,0.0006616801,0.0003114096,0.00022498584,0.00273306],"category_scores_gemma":[0.00089001225,0.00023537157,0.00021945316,0.0010507321,0.00032924465,0.0002960765,0.0006902902,0.00031933023,0.0011370779],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005261449,0.00006384725,0.8641253,0.00011578942,0.0001585893,0.0003461125,0.0010128457,0.0029198553,0.07834783,0.00084240205,0.013791197,0.037750095],"study_design_scores_gemma":[0.000005673132,0.0000059489194,0.99683124,0.000004460943,0.000008957236,0.000033848515,0.000040503797,0.00058135326,0.0011811071,0.00013736014,0.0011634025,0.0000062682525],"about_ca_topic_score_codex":0.016031306,"about_ca_topic_score_gemma":0.025643164,"teacher_disagreement_score":0.016031306,"about_ca_system_score_codex":0.00043056547,"about_ca_system_score_gemma":0.00019706643,"threshold_uncertainty_score":0.031875968},"labels":[],"label_agreement":null},{"id":"W4200011565","doi":"10.3847/1538-4357/ac3137","title":"New Perspectives on the Exoplanet Radius Gap from a Mathematica Tool and Visualized Water Equation of State","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Exoplanet; Planet; RADIUS; Astrobiology; Equation of state; Physics; Astrophysics; Earth radius; Thermodynamics","score_opus":0.02030169765830893,"score_gpt":0.24852864734275615,"score_spread":0.22822694968444723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200011565","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0333283,0.00036935927,0.95464015,0.0007517057,0.00006775289,0.000020374286,0.00060789095,0.003739572,0.0064749075],"genre_scores_gemma":[0.3862916,0.00063391845,0.60764116,0.00015977742,0.00007419754,0.00014492041,0.00081496243,0.0019182701,0.0023211124],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999668,0.0001255936,0.000025093315,0.00007724009,0.00007343374,0.000030623643],"domain_scores_gemma":[0.9986663,0.0008945994,0.0001303023,0.00012747796,0.00011056724,0.00007067205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010257653,0.0008798443,0.00064791855,0.0025545962,0.00052777614,0.002304213,0.00090604584,0.00047422302,0.008873788],"category_scores_gemma":[0.004239415,0.00036297724,0.0011723874,0.0016573131,0.0011382647,0.0029899247,0.0021249824,0.0013043911,0.00082859024],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012186473,0.000058412596,0.004374772,0.00033817693,0.00005342644,0.0007427249,0.0025786823,0.079690926,0.009164897,0.8354494,0.0069234297,0.060503226],"study_design_scores_gemma":[0.00002743933,0.000039210747,0.0011596802,0.000081009115,0.000025696236,0.00032377683,0.0004487478,0.56127197,0.0043070996,0.3792281,0.053033434,0.000053865297],"about_ca_topic_score_codex":0.0019476884,"about_ca_topic_score_gemma":0.00090757344,"teacher_disagreement_score":0.008873788,"about_ca_system_score_codex":0.00064026815,"about_ca_system_score_gemma":0.0003797864,"threshold_uncertainty_score":0.029685795},"labels":[],"label_agreement":null},{"id":"W4200013041","doi":"10.3847/1538-4357/ac25ec","title":"Energy-dependent Boundaries of Earth's Radiation Belt Electron Slot Region","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Memorial University of Newfoundland","funders":"National Natural Science Foundation of China","keywords":"Physics; Van Allen radiation belt; Magnetosphere; Electron; Saturn; Jupiter (rocket family); Geophysics; Computational physics; Earth's magnetic field; Solar wind; Planet; Astrophysics; Magnetic field; Astronomy; Plasma; Nuclear physics; Spacecraft","score_opus":0.004357534948317789,"score_gpt":0.20266662591019619,"score_spread":0.1983090909618784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200013041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98069084,0.0001764723,0.014784387,0.00009417189,0.000010089568,0.000012339723,0.0006093171,0.000188304,0.0034341912],"genre_scores_gemma":[0.9992526,0.000026799551,0.00037577446,0.0000050350304,0.0000012997904,0.000004554431,0.00012778828,0.000015641346,0.00019042578],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999231,0.000011630606,0.0000041085914,0.00003354923,0.000009840803,0.000017804152],"domain_scores_gemma":[0.9997316,0.00009117341,0.00007311276,0.000041813822,0.00003773679,0.000024622865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024860053,0.00020900046,0.00022141407,0.0003309639,0.00018050412,0.00060483103,0.00069951784,0.00048756634,0.001312734],"category_scores_gemma":[0.001340074,0.00021610165,0.00034758862,0.00023184597,0.00042875105,0.00093711104,0.00035185498,0.00032825646,0.00018255503],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017391793,0.000030451223,0.0676083,0.000053574455,0.000037100916,0.00013941605,0.00013374462,0.90738124,0.012869389,0.0060784426,0.0004859108,0.005008478],"study_design_scores_gemma":[0.000018663573,0.000029539993,0.04193115,0.000017200317,0.000012419798,0.00006526726,0.00007717996,0.95073515,0.0034769776,0.0026661886,0.00094736397,0.000022937067],"about_ca_topic_score_codex":0.009350645,"about_ca_topic_score_gemma":0.0035412163,"teacher_disagreement_score":0.009350645,"about_ca_system_score_codex":0.0007068433,"about_ca_system_score_gemma":0.00028982494,"threshold_uncertainty_score":0.018592477},"labels":[],"label_agreement":null},{"id":"W4200013606","doi":"10.3847/1538-4357/ac2948","title":"On the Properties of Spectroscopically Confirmed Ultra-diffuse Galaxies across Environments","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; University of Arizona; National Science Foundation","keywords":"Galaxy; Coma Cluster; Physics; Astrophysics; Redshift; Cluster (spacecraft); RADIUS; Galaxy cluster; Astronomy; Computer science","score_opus":0.010609875595601519,"score_gpt":0.21188197245509832,"score_spread":0.2012720968594968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200013606","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99935955,0.00005491219,0.00013917788,0.0000035398514,5.4973384e-7,0.0000022461409,0.00008568108,0.000008417026,0.00034599984],"genre_scores_gemma":[0.9996176,0.000017055068,0.0001318759,0.0000036992424,0.0000011429933,0.0000014030219,0.00016674411,0.0000017408,0.00005861391],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974555,0.000040005812,0.000017537686,0.00006326644,0.00007117885,0.00006253902],"domain_scores_gemma":[0.9984415,0.00022203905,0.00062266627,0.00019090356,0.00021693172,0.00030593618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035823337,0.0002309608,0.00024225202,0.0020201788,0.00032563446,0.0005621168,0.00035328465,0.00015885131,0.0010750387],"category_scores_gemma":[0.0012707841,0.00011369128,0.00017569966,0.0009841757,0.00040155603,0.00025133867,0.00088775204,0.00012699906,0.00024834726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055889173,0.0000102803415,0.9920952,0.000008603592,0.000013466401,0.000042892647,0.00015559484,0.00006365608,0.0039261607,0.00006187182,0.000040209383,0.0035262178],"study_design_scores_gemma":[8.858193e-7,0.00002044744,0.9991597,0.0000019213455,0.0000048426286,0.00008740893,0.00014678348,0.00007372414,0.00036187522,0.000015574178,0.00012574373,0.0000011444773],"about_ca_topic_score_codex":0.0029752688,"about_ca_topic_score_gemma":0.006914075,"teacher_disagreement_score":0.0029752688,"about_ca_system_score_codex":0.00020935942,"about_ca_system_score_gemma":0.00009084102,"threshold_uncertainty_score":0.00591588},"labels":[],"label_agreement":null},{"id":"W4200084571","doi":"10.3847/1538-4357/ac22a6","title":"Eta Carinae: A Tale of Two Periastron Passages","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Astronomy; Flux (metallurgy); Space Telescope Imaging Spectrograph; Spectrograph; Wavelength; Supergiant; Spectral line; Stars; Hubble space telescope; Optics","score_opus":0.010544156180741313,"score_gpt":0.23951735345571337,"score_spread":0.22897319727497206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200084571","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96216184,0.004222991,0.00065705116,0.0036438308,0.00075216603,0.000043131848,0.00046247753,0.00010767543,0.027948711],"genre_scores_gemma":[0.9886268,0.0010411496,0.00054880796,0.0005757423,0.0003774073,0.000012848072,0.00051157596,0.00003594109,0.008269921],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997943,0.000024826537,0.000009343948,0.000060846924,0.00005308459,0.00005764729],"domain_scores_gemma":[0.99962616,0.00004911206,0.000080439175,0.00003845604,0.00006917303,0.00013668076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034384176,0.0003211027,0.00023503361,0.0010013932,0.0033565145,0.0019359629,0.00045779592,0.0010721029,0.0042962213],"category_scores_gemma":[0.0008286388,0.00016773574,0.00026627394,0.00069693825,0.0009264863,0.0013146175,0.0020447576,0.0011417185,0.0009007916],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0027293426,0.0003924103,0.49879158,0.0007460117,0.00030085593,0.05341484,0.1010881,0.0009880608,0.048554406,0.013441246,0.040770147,0.23878299],"study_design_scores_gemma":[0.000020941436,0.00031042122,0.75775504,0.0002237194,0.00004637225,0.010908773,0.024662798,0.00034354813,0.002036731,0.0024158242,0.20119883,0.000077069555],"about_ca_topic_score_codex":0.0041779666,"about_ca_topic_score_gemma":0.008844646,"teacher_disagreement_score":0.0042962213,"about_ca_system_score_codex":0.00093465217,"about_ca_system_score_gemma":0.0002167936,"threshold_uncertainty_score":0.014372289},"labels":[],"label_agreement":null},{"id":"W4200149132","doi":"10.3847/1538-4357/ac2bfe","title":"Ubiquitous [O ii] Emission in Quiescent Galaxies at z ≈ 0.85 from the LEGA-C Survey*","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"European Research Council; Science and Technology Facilities Council; European Commission","keywords":"Physics; Galaxy; Astrophysics; Astronomy; Emission spectrum; Spectral line","score_opus":0.011415962953672148,"score_gpt":0.22095043419817953,"score_spread":0.2095344712445074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200149132","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982351,0.00010932102,0.00004333735,0.000028149956,0.0000018154943,0.0000031264935,0.0008335822,0.000012160143,0.0007334264],"genre_scores_gemma":[0.9972168,0.00006335504,0.00011625857,0.00005394185,0.0000062408058,0.0000033234592,0.0023654923,0.000004538036,0.00017000329],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980766,0.000019595705,0.000013095773,0.00006008833,0.000031337324,0.00006818745],"domain_scores_gemma":[0.99912137,0.00007261555,0.00029612723,0.00008131409,0.00008691848,0.00034166014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028287398,0.00027790057,0.00025936292,0.0019139762,0.00040907893,0.0011029379,0.00031651053,0.00027812668,0.0012134758],"category_scores_gemma":[0.0005514562,0.00013366425,0.00023512148,0.0010767746,0.00032987303,0.0002649485,0.000658154,0.00019219726,0.00043314914],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051540555,0.000017410084,0.9934638,0.000011065118,0.00003245477,0.000052238047,0.00014642197,0.000027143315,0.0038485865,0.00004902679,0.00021375195,0.0020865418],"study_design_scores_gemma":[0.0000014583177,0.000007550419,0.9995993,0.0000023420284,0.000006069646,0.00003058109,0.00004641214,0.000032281074,0.00007260935,0.000008295898,0.00019206134,0.0000010271982],"about_ca_topic_score_codex":0.015671628,"about_ca_topic_score_gemma":0.02883807,"teacher_disagreement_score":0.015671628,"about_ca_system_score_codex":0.00036365076,"about_ca_system_score_gemma":0.00018029977,"threshold_uncertainty_score":0.031160831},"labels":[],"label_agreement":null},{"id":"W4200186752","doi":"10.3847/1538-4357/ac1442","title":"MOMO. IV. The Complete Swift X-Ray and UV/Optical Light Curve and Characteristic Variability of the Blazar OJ 287 during the Last Two Decades","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Light curve; Blazar; Astrophysics; Flare; Jet (fluid); Swift; Superluminal motion; Astronomy; Gamma ray","score_opus":0.0065156348304207575,"score_gpt":0.2100988237435908,"score_spread":0.20358318891317004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200186752","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97708344,0.0007175213,0.00093761313,0.0001193684,0.000037168644,0.000033029417,0.01257393,0.00023022052,0.008267812],"genre_scores_gemma":[0.9685563,0.00024766038,0.0010646292,0.00007307894,0.00006866631,0.000019504514,0.026743853,0.0001296714,0.003096592],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992657,0.0000024868389,0.0000037589343,0.000019923524,0.0000251061,0.000022059136],"domain_scores_gemma":[0.99968946,0.000012481973,0.00010990459,0.000037444184,0.000054916436,0.00009587211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020272778,0.00023852648,0.00019173545,0.0007139059,0.000267206,0.0007331186,0.00016970145,0.00013427551,0.0012199408],"category_scores_gemma":[0.0002747348,0.000108021435,0.00019040516,0.0005135356,0.00014780168,0.00020004933,0.00041474568,0.0002530005,0.0007750102],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000751134,0.00033647957,0.851654,0.00032447642,0.00016109568,0.0012016293,0.00072276546,0.0020848473,0.04061114,0.0010740445,0.014783987,0.086294435],"study_design_scores_gemma":[0.000012772583,0.000048608028,0.98647565,0.000013878121,0.000020474903,0.00016663237,0.00007215915,0.000860518,0.0015585194,0.00009649249,0.010667838,0.000006480755],"about_ca_topic_score_codex":0.009296485,"about_ca_topic_score_gemma":0.010443332,"teacher_disagreement_score":0.009296485,"about_ca_system_score_codex":0.00030845214,"about_ca_system_score_gemma":0.00035592183,"threshold_uncertainty_score":0.018484712},"labels":[],"label_agreement":null},{"id":"W4200344202","doi":"10.3847/1538-4357/ac142b","title":"The Green Bank Northern Celestial Cap Pulsar Survey. VI. Discovery and Timing of PSR J1759+5036: A Double Neutron Star Binary Pulsar","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Science and Technology Facilities Council; National Science Foundation","keywords":"Pulsar; Physics; Millisecond pulsar; Neutron star; Astrophysics; Binary pulsar; Green Bank Telescope; Pulsar planet; X-ray pulsar; Astronomy; Orbital period; White dwarf; Radio telescope; Stars","score_opus":0.019734459235533543,"score_gpt":0.30073708823875867,"score_spread":0.28100262900322515,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200344202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9552883,0.0014093465,0.0002028938,0.00049678725,0.00007259843,0.000080200036,0.027320476,0.00010064539,0.015028712],"genre_scores_gemma":[0.96745276,0.0012644769,0.0013668879,0.0004305482,0.00009699422,0.0000633767,0.020872414,0.000042690914,0.008409796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997416,0.000040373987,0.000023304181,0.000053878022,0.000093444134,0.00004730873],"domain_scores_gemma":[0.99880457,0.00006613629,0.0003190263,0.00009944418,0.00029763585,0.00041320952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004937292,0.00020047819,0.00028369098,0.0023995256,0.00073175057,0.00053196785,0.00026888965,0.00021284189,0.0030823601],"category_scores_gemma":[0.0006253744,0.00016741168,0.0001131148,0.0021016162,0.00025109915,0.00022834093,0.000600839,0.00019427501,0.0014624232],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038526196,0.000057409092,0.95236534,0.000083219566,0.000048588736,0.00064129644,0.000329865,0.00017636122,0.0047050454,0.0002344804,0.019531665,0.021441516],"study_design_scores_gemma":[0.000012368984,0.000020969519,0.99355716,0.0000145288595,0.0000066886473,0.00015635078,0.00009456315,0.00012985493,0.00025564016,0.000018227931,0.0057294816,0.0000042448173],"about_ca_topic_score_codex":0.23903456,"about_ca_topic_score_gemma":0.4080036,"teacher_disagreement_score":0.23903456,"about_ca_system_score_codex":0.0011841524,"about_ca_system_score_gemma":0.0011783212,"threshold_uncertainty_score":0.47528648},"labels":[],"label_agreement":null},{"id":"W4200374503","doi":"10.3847/1538-4357/ac2499","title":"A Wide Planetary Mass Companion Discovered through the Citizen Science Project Backyard Worlds: Planet 9","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Planet; Brown dwarf; Astrophysics; Photometry (optics); Parallax; Astronomy; Proper motion; Planetary mass; Primary (astronomy); Stellar classification; Planetary system; Spectral line; Stars","score_opus":0.017317365781104908,"score_gpt":0.24656165516606748,"score_spread":0.22924428938496258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200374503","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9080128,0.0002546196,0.0027049202,0.002709574,0.00010506344,0.00021345005,0.0427463,0.0004390136,0.04281422],"genre_scores_gemma":[0.93628144,0.0002010813,0.005727228,0.00052483665,0.000077726734,0.00016457497,0.037838206,0.000106490304,0.019078573],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99940836,0.000074398944,0.000027455197,0.000119774675,0.00021274966,0.00015728462],"domain_scores_gemma":[0.9978265,0.0001569331,0.00044493587,0.0003432078,0.00055054226,0.0006778211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009083755,0.00015680882,0.00020102065,0.0015250623,0.0014197606,0.00088596786,0.00035925614,0.00040027688,0.007549238],"category_scores_gemma":[0.0021487807,0.00011716689,0.00017726666,0.0018814971,0.0002917734,0.00084256567,0.0030104895,0.0004944389,0.0023944667],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023546428,0.0002651512,0.7845656,0.00015590586,0.000043476,0.0017464869,0.004800593,0.00014707279,0.008771504,0.0024710852,0.08464969,0.11214793],"study_design_scores_gemma":[0.000016079186,0.000112421425,0.74601704,0.00006417184,0.000024495956,0.001726225,0.0037970885,0.00050912297,0.0031891777,0.0010627704,0.2434581,0.000023379378],"about_ca_topic_score_codex":0.014457382,"about_ca_topic_score_gemma":0.022664601,"teacher_disagreement_score":0.014457382,"about_ca_system_score_codex":0.0004474709,"about_ca_system_score_gemma":0.00094295916,"threshold_uncertainty_score":0.028746426},"labels":[],"label_agreement":null},{"id":"W4200423632","doi":"10.3847/1538-4357/ac4267","title":"Erratum: “A Gravitational-wave Measurement of the Hubble Constant Following the Second Observing Run of Advanced LIGO and Virgo” (2021, ApJ, 909, 218)","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal","funders":"Science and Technology Facilities Council","keywords":"LIGO; Physics; Gravitational wave; Astronomy; Hubble's law; Astrophysics; Galaxy; Redshift","score_opus":0.014029044060161132,"score_gpt":0.23545640657614503,"score_spread":0.22142736251598388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200423632","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0010679408,0.0018351673,0.0003449366,0.082246415,0.8741829,0.000041998057,0.007358648,0.0004256684,0.03249631],"genre_scores_gemma":[0.014178378,0.0052299323,0.0024121185,0.111405954,0.11798085,0.00016846617,0.014936056,0.0010612811,0.73262703],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99853253,0.000148161,0.00027368413,0.00022452905,0.00067544077,0.00014571019],"domain_scores_gemma":[0.99339163,0.0014588463,0.00041592604,0.0003709416,0.0038588932,0.00050378096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014957464,0.0019533695,0.0011884742,0.0029878884,0.005097646,0.0036889215,0.0018387125,0.0054063895,0.041492492],"category_scores_gemma":[0.012757241,0.0008308337,0.00090717705,0.0017811846,0.0009803122,0.0021683543,0.0014623314,0.006364038,0.0443359],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037554113,0.000009283814,0.00011835034,0.000038160753,0.0000032680878,0.00015397626,0.000016108535,0.000028170301,0.00005800099,0.00043184453,0.9966718,0.0024334162],"study_design_scores_gemma":[0.000035130288,0.000037636928,0.0053458693,0.00023896614,0.000025053288,0.00029948523,0.00017676085,0.00018491813,0.00045959538,0.0012274977,0.9919208,0.000048162194],"about_ca_topic_score_codex":0.052267388,"about_ca_topic_score_gemma":0.0875804,"teacher_disagreement_score":0.052267388,"about_ca_system_score_codex":0.0036977404,"about_ca_system_score_gemma":0.004886136,"threshold_uncertainty_score":0.13880622},"labels":[],"label_agreement":null},{"id":"W4200460017","doi":"10.3847/1538-4357/ac28fc","title":"The 6.2 μm PAH Feature and the Role of Nitrogen: Revisited","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Science Mission Directorate","keywords":"Physics; Spectral line; Astrophysics; Infrared; Polarization (electrochemistry); Nitrogen; Protonation; Ion; Astronomy; Physical chemistry; Chemistry; Quantum mechanics","score_opus":0.0037487822359675263,"score_gpt":0.20881597818767855,"score_spread":0.20506719595171102,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200460017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9938595,0.00022458202,0.0032823817,0.000039808947,0.0000057091124,0.00000348677,0.00012257717,0.00006228316,0.002399655],"genre_scores_gemma":[0.9991648,0.00005795707,0.0005877882,0.000009384899,0.0000023196403,9.028499e-7,0.00005719369,0.000007911633,0.00011186794],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992645,0.000011304599,0.0000021877272,0.00002006116,0.00002458294,0.00001542467],"domain_scores_gemma":[0.9998816,0.000036509235,0.000024731246,0.000022150263,0.000024149409,0.000010824661],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014624611,0.00031194714,0.0001498127,0.00022979728,0.00016572133,0.00030588126,0.0005026749,0.00028805804,0.00081722625],"category_scores_gemma":[0.00038923632,0.000117338626,0.00016747044,0.00025566618,0.00025722585,0.00045447273,0.00026547266,0.0002129779,0.00013190079],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000640948,0.0001693613,0.24477382,0.00037957984,0.0002393558,0.0014780156,0.00024698602,0.2561671,0.42325476,0.012108305,0.000861742,0.059679992],"study_design_scores_gemma":[0.000044655848,0.00032701713,0.23742299,0.000050957642,0.00010151123,0.0007108086,0.0003084549,0.60451186,0.14386077,0.008108369,0.0044992957,0.00005321951],"about_ca_topic_score_codex":0.0018981573,"about_ca_topic_score_gemma":0.0018421157,"teacher_disagreement_score":0.0018981573,"about_ca_system_score_codex":0.000208082,"about_ca_system_score_gemma":0.00010178006,"threshold_uncertainty_score":0.0037742257},"labels":[],"label_agreement":null},{"id":"W4200494635","doi":"10.3847/1538-4357/ac02bb","title":"Optimal Cosmic Microwave Background Lensing Reconstruction and Parameter Estimation with SPTpol Data","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":54,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"Office of Science; Argonne National Laboratory; National Energy Research Scientific Computing Center; High Energy Physics; Gordon and Betty Moore Foundation; U.S. Department of Energy; University of Chicago; National Science Foundation","keywords":"Cosmic microwave background; Physics; Amplitude; Algorithm; Astrophysics; Optics; Anisotropy; Computer science","score_opus":0.020819316924268035,"score_gpt":0.26155968643158767,"score_spread":0.24074036950731964,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200494635","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.67164654,0.00018563578,0.31906712,0.0006268197,0.000029795205,0.00004738005,0.0022534067,0.0022249245,0.0039184615],"genre_scores_gemma":[0.84400237,0.000059336715,0.14952673,0.0001021648,0.000027483175,0.00004582935,0.0050707306,0.00051355787,0.0006517364],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99873406,0.0005039954,0.000044016284,0.00023506726,0.00031195334,0.00017087715],"domain_scores_gemma":[0.9973115,0.0012193611,0.0002756174,0.00059136515,0.0004554731,0.00014676675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002295257,0.0007839559,0.000812023,0.0010773045,0.00057688163,0.0018060672,0.0012479704,0.0012361276,0.0016292902],"category_scores_gemma":[0.011998387,0.001006552,0.00092967146,0.0011293644,0.0008964391,0.0014431758,0.0014317858,0.001250908,0.00078859046],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013190008,0.00030688723,0.057071973,0.00018901654,0.00045468542,0.0004574216,0.0004017624,0.8005763,0.026862593,0.019388784,0.00499037,0.08798119],"study_design_scores_gemma":[0.00014185949,0.00005818499,0.014003719,0.000017064367,0.000043425374,0.0000657741,0.000083506384,0.9631623,0.01010466,0.010734096,0.0015156077,0.000069712994],"about_ca_topic_score_codex":0.0096448595,"about_ca_topic_score_gemma":0.010676847,"teacher_disagreement_score":0.0096448595,"about_ca_system_score_codex":0.00074383256,"about_ca_system_score_gemma":0.0015268852,"threshold_uncertainty_score":0.019177437},"labels":[],"label_agreement":null},{"id":"W4200551697","doi":"10.3847/1538-4357/ac1ff7","title":"Quasi-simultaneous Radio/X-Ray Observations of the Candidate Transitional Millisecond Pulsar 3FGL J1544.6−1125 during its Low-luminosity Accretion-disk State","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Astrophysics Division; Astrophysics Science Division; Smithsonian Astrophysical Observatory; European Commission; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Goddard Space Flight Center; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Pulsar; Millisecond pulsar; Luminosity; Accretion (finance); Neutron star; Astronomy; Galaxy","score_opus":0.010524885268782817,"score_gpt":0.2153722358182018,"score_spread":0.204847350549419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200551697","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985012,0.000059661324,0.00015282551,0.00001698547,0.0000055585256,0.000009867057,0.00039318632,0.00002735089,0.00083338504],"genre_scores_gemma":[0.99735343,0.00003061259,0.0004940042,0.000031679756,0.000017115717,0.00001689537,0.0015206632,0.000009965036,0.000525661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987495,0.000011164492,0.0000057825473,0.000042004765,0.000026185902,0.000039785624],"domain_scores_gemma":[0.99972516,0.000023725855,0.00006604099,0.000024594263,0.000035835597,0.0001246515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026837637,0.00027476152,0.000340873,0.0010488079,0.0006631194,0.00048308773,0.0003694716,0.0003125756,0.001478623],"category_scores_gemma":[0.00020671063,0.00018173737,0.00025824318,0.0004403176,0.00021184214,0.00016919589,0.0005172397,0.00032268284,0.00036828898],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012132234,0.00035009076,0.7673987,0.00007382661,0.00017259092,0.001284807,0.00065245706,0.0005124375,0.2089827,0.00014718666,0.0010166815,0.018195223],"study_design_scores_gemma":[0.000008896082,0.00013275613,0.99760395,0.0000034588875,0.000018649755,0.00015756252,0.000092472386,0.00013397087,0.0012557602,0.000010513583,0.0005775012,0.000004529458],"about_ca_topic_score_codex":0.0042946753,"about_ca_topic_score_gemma":0.014460657,"teacher_disagreement_score":0.0042946753,"about_ca_system_score_codex":0.00033715912,"about_ca_system_score_gemma":0.00016353611,"threshold_uncertainty_score":0.008539319},"labels":[],"label_agreement":null},{"id":"W4200632599","doi":"10.3847/1538-4357/ac61df","title":"An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Survey Description and First Results","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Ministry of Science and Technology, Taiwan","keywords":"Physics; Astronomy; Galaxy; Astrophysics; Luminous infrared galaxy; James Clerk Maxwell Telescope; Cosmos (plant); Star formation","score_opus":0.016491874411923638,"score_gpt":0.22484680398569867,"score_spread":0.20835492957377505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200632599","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872114,0.00017037857,0.00091002986,0.000036609716,0.0000036550948,0.000074514064,0.009702186,0.00013870384,0.001752398],"genre_scores_gemma":[0.9714726,0.00016692026,0.0038957526,0.00006698083,0.00004000504,0.00012899163,0.022901196,0.000040846546,0.0012867692],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99963105,0.00007416882,0.000024290659,0.000081429534,0.00010767516,0.00008134013],"domain_scores_gemma":[0.998672,0.000111460686,0.00028041477,0.00018665157,0.0003110054,0.00043852266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006528253,0.00052204815,0.0002462183,0.0033352044,0.00036459562,0.00053174555,0.00037643578,0.00024150206,0.0019160095],"category_scores_gemma":[0.000677477,0.00020030527,0.00030217637,0.0020568958,0.00016281914,0.00033906847,0.0006506354,0.00017878505,0.0010296479],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008931702,0.00006998316,0.98649085,0.000025554587,0.000037694943,0.00006016963,0.00009248028,0.00013426998,0.0047717476,0.00006466497,0.0012872971,0.0068759797],"study_design_scores_gemma":[0.0000101314035,0.00003368588,0.9974718,0.000003964307,0.000012208015,0.00006168873,0.000054996064,0.0004215782,0.00069373654,0.0000171964,0.0012148105,0.000004180631],"about_ca_topic_score_codex":0.015438318,"about_ca_topic_score_gemma":0.02446049,"teacher_disagreement_score":0.015438318,"about_ca_system_score_codex":0.00035438314,"about_ca_system_score_gemma":0.00042647755,"threshold_uncertainty_score":0.030696929},"labels":[],"label_agreement":null},{"id":"W4200633136","doi":"10.3847/1538-4357/ac69d4","title":"Searching for Anomalies in the ZTF Catalog of Periodic Variable Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Astronomical Sciences","keywords":"Physics; Stars; Variable star; Astrophysics; Milky Way; Astronomy; Variable (mathematics); Stellar dynamics","score_opus":0.013878222614681551,"score_gpt":0.23701118120118522,"score_spread":0.22313295858650367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200633136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98807096,0.00013445261,0.0038031035,0.00012549032,0.000009278733,0.000018902383,0.0062334677,0.0004357004,0.0011686325],"genre_scores_gemma":[0.97264713,0.000077262564,0.005660734,0.000021604761,0.0000205702,0.000014194838,0.021056343,0.00004201694,0.00046020828],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971205,0.000020885269,0.00002342124,0.00007104416,0.00010615766,0.000066365086],"domain_scores_gemma":[0.99840087,0.00023834544,0.0005137271,0.0002769025,0.00037703651,0.00019314913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005907926,0.00014057686,0.00022536886,0.0052981493,0.0003732675,0.0006653132,0.0004252513,0.00038038517,0.0010032248],"category_scores_gemma":[0.002283128,0.0000884898,0.00018628899,0.0029976561,0.0002409866,0.00055284397,0.0006859792,0.00025473523,0.0005577751],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001080105,0.000051389678,0.927287,0.00003859646,0.000033358425,0.00016728866,0.00015709472,0.0036483647,0.0075030336,0.0011968872,0.0053783604,0.054430682],"study_design_scores_gemma":[0.00001724894,0.000048506776,0.9239711,0.000021159658,0.000022731632,0.0003543581,0.0002097637,0.062249955,0.0035699268,0.0013836195,0.008132636,0.000019062454],"about_ca_topic_score_codex":0.0074425475,"about_ca_topic_score_gemma":0.011202941,"teacher_disagreement_score":0.0074425475,"about_ca_system_score_codex":0.00038561813,"about_ca_system_score_gemma":0.00052641134,"threshold_uncertainty_score":0.014798403},"labels":[],"label_agreement":null},{"id":"W4200633280","doi":"10.3847/1538-4357/ac400d","title":"A Comparison of Multiphase Magnetic Field Tracers in a High Galactic Latitude Region of the Filamentary Interstellar Medium","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Magnetic field; Astrophysics; Interstellar medium; Galactic plane; Polarization (electrochemistry); Plasma; Field line; Molecular cloud; Ionization; Astronomy; Galaxy; Stars; Ion","score_opus":0.014545469136700358,"score_gpt":0.26425594249688944,"score_spread":0.2497104733601891,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200633280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985719,0.00010211326,0.00047631105,0.000012280761,0.00000177971,0.000004391428,0.00022252109,0.00003439675,0.0005742047],"genre_scores_gemma":[0.9989293,0.000050951214,0.0005946575,0.0000056266467,0.000005924803,0.0000037780494,0.00031651402,0.000005653374,0.00008748501],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999335,0.0000056559225,0.0000035588341,0.000023556815,0.000014367099,0.00001934529],"domain_scores_gemma":[0.9996679,0.000042530144,0.00015416248,0.000023725537,0.000050455244,0.00006122524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014250372,0.00019953499,0.00017389513,0.0016206307,0.00021191829,0.00062562333,0.0002785109,0.00026041377,0.0006931036],"category_scores_gemma":[0.00039114323,0.00012806764,0.00014047061,0.00075328647,0.00016159324,0.00031991405,0.00037899704,0.000120991695,0.00012544106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037341678,0.0000739295,0.8233838,0.00007002035,0.00014923862,0.00029198432,0.00027173408,0.0020834128,0.15786056,0.00033607878,0.00023569838,0.014870211],"study_design_scores_gemma":[0.000008087036,0.000034658915,0.99284464,0.0000081450235,0.00002217371,0.000106753505,0.00009637838,0.002470874,0.003934894,0.00007166551,0.0003962922,0.000005485997],"about_ca_topic_score_codex":0.002711445,"about_ca_topic_score_gemma":0.0036765712,"teacher_disagreement_score":0.002711445,"about_ca_system_score_codex":0.00026417463,"about_ca_system_score_gemma":0.00007799529,"threshold_uncertainty_score":0.0053913593},"labels":[],"label_agreement":null},{"id":"W4200635217","doi":"10.3847/1538-4357/ac4270","title":"WALLABY Pre-pilot Survey: The Effects of Tidal Interaction on Radial Distribution of Color in Galaxies of the Eridanus Supergroup","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Ministry of Science and ICT, South Korea; Division of Astronomical Sciences; Jet Propulsion Laboratory; Office of Science; Peking University; Chinese Academy of Sciences; U.S. Department of Energy; National Natural Science Foundation of China; High Energy Physics; Deutsche Forschungsgemeinschaft; Science and Technology Facilities Council; National Aeronautics and Space Administration; University College London; Ohio State University; National Research Foundation; University of Sussex; National Research Foundation of Korea; University of Portsmouth; University of Chicago; University of Illinois at Urbana-Champaign; California Institute of Technology; Fermilab; National Science Foundation","keywords":"Astrophysics; Physics; Galaxy; Sky; Asymmetry; Astronomy","score_opus":0.006398244555804458,"score_gpt":0.21022977998582704,"score_spread":0.20383153543002258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200635217","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99962485,0.000010106032,0.00001763263,0.0000036483448,2.7815307e-7,8.8280694e-7,0.00009449059,0.0000018303142,0.00024636407],"genre_scores_gemma":[0.9994814,0.000008416374,0.00003533613,0.0000027664676,0.0000010538639,0.00000153582,0.00028135406,0.0000018232923,0.00018633275],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998258,0.000028729748,0.000010104777,0.000051010218,0.000035307876,0.000049089227],"domain_scores_gemma":[0.9991842,0.00009657732,0.00027603173,0.0000910658,0.00009242607,0.00025969362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029995188,0.00015805493,0.00021771334,0.0007777695,0.0002713108,0.0003207126,0.00022129694,0.00015738208,0.0014102148],"category_scores_gemma":[0.00074449775,0.00009614256,0.00012158304,0.0004408562,0.00026003664,0.00023856651,0.0006795566,0.00010394616,0.0003062577],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000085697684,0.000014031623,0.9938444,0.0000040277337,0.000012380315,0.00005075159,0.00020751692,0.00007863882,0.0037167044,0.000030523275,0.000052180563,0.0019031385],"study_design_scores_gemma":[4.952728e-7,0.0000074736304,0.99980646,4.84987e-7,0.0000011995146,0.000007502581,0.00005329778,0.000034927914,0.00004903358,0.0000018156627,0.00003684148,4.2495287e-7],"about_ca_topic_score_codex":0.018108806,"about_ca_topic_score_gemma":0.032006104,"teacher_disagreement_score":0.018108806,"about_ca_system_score_codex":0.00021865946,"about_ca_system_score_gemma":0.00015784001,"threshold_uncertainty_score":0.03600681},"labels":[],"label_agreement":null},{"id":"W4200635822","doi":"10.3847/1538-4357/ac5b60","title":"SOAR/Goodman Spectroscopic Assessment of Candidate Counterparts of the LIGO/Virgo Event GW190814*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; University of North Carolina at Chapel Hill; Office of Science; Australian Research Council; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Ministerio de Ciencia e Innovación; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Israel Science Foundation; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Council for Higher Education; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministerio de Economía y Competitividad; Ministério da Ciência, Tecnologia e Inovação; Fundação de Amparo à Pesquisa do Estado de São Paulo; University of Portsmouth; Kavli Institute for Cosmological Physics, University of Chicago; United States-Israel Binational Science Foundation; Canadian Institute for Advanced Research; Fraternal Order of Eagles; University College London; National Aeronautics and Space Administration; Lawrence Berkeley National Laboratory; Financiadora de Estudos e Projetos; University of Pennsylvania; Institut de Física d'Altes Energies; Eidgenössische Technische Hochschule Zürich; National Centre for Supercomputing Applications; University of Illinois at Urbana-Champaign; Michigan State University; College of Engineering, Michigan State University; Brinson Foundation; Ohio State University; University of California, Santa Cruz; U.S. Department of Energy; Center for Cosmology and Astroparticle Physics, Ohio State University; University of Sussex; Heising-Simons Foundation; Gordon and Betty Moore Foundation; High Energy Physics; Deutsche Forschungsgemeinschaft; David and Lucile Packard Foundation; Fermilab; National Science Foundation","keywords":"LIGO; Soar; Event (particle physics); Astronomy; Computer science; Physics; Astrophysics; Artificial intelligence; Gravitational wave","score_opus":0.006665364525169471,"score_gpt":0.2531112622935455,"score_spread":0.24644589776837605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4200635822","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970343,0.00002487195,0.0001707447,0.000054252698,0.0000048505144,0.000015135041,0.00023975017,0.00002609834,0.0024298423],"genre_scores_gemma":[0.9977575,0.00002281576,0.00072908954,0.00003658536,0.000010835082,0.0000084581825,0.0007664621,0.000013615963,0.0006547116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997967,0.000022974427,0.00001034367,0.000053591906,0.000050171384,0.00006625168],"domain_scores_gemma":[0.99935347,0.00005162763,0.00021611407,0.000078113015,0.00011213359,0.00018857411],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066208094,0.00015815532,0.00018142466,0.0016710199,0.00061329827,0.00043889534,0.00027800712,0.00019339785,0.0017656973],"category_scores_gemma":[0.0007377652,0.0001134553,0.00017446297,0.0004926689,0.00026168785,0.0002493471,0.0006520026,0.00023348488,0.00035399533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039086354,0.00009617085,0.94722515,0.00001618997,0.000037859252,0.00081206096,0.0006397975,0.00012456263,0.03722932,0.00029055073,0.0012680355,0.011869447],"study_design_scores_gemma":[0.000007165217,0.00008736567,0.996135,0.000003137514,0.000009027379,0.00023255468,0.00022180156,0.00026217714,0.0017843344,0.000053454685,0.0011989404,0.000005022567],"about_ca_topic_score_codex":0.0048729847,"about_ca_topic_score_gemma":0.012469696,"teacher_disagreement_score":0.0048729847,"about_ca_system_score_codex":0.0003984487,"about_ca_system_score_gemma":0.00018117453,"threshold_uncertainty_score":0.009689212},"labels":[],"label_agreement":null},{"id":"W4205352972","doi":"10.3847/1538-4357/abaabb","title":"Erratum: “Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015–2017 LIGO Data” (2019, ApJ, 879, 10)","year":2020,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"LIGO; Physics; Gravitational wave; Pulsar; Astronomy; Astrophysics; Einstein Telescope; Harmonics; Gravitational-wave observatory; Quantum mechanics","score_opus":0.0538111061349571,"score_gpt":0.3704571437244842,"score_spread":0.3166460375895271,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4205352972","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0015121056,0.00169964,0.0022981677,0.050673123,0.88218564,0.000051235696,0.033363417,0.0023619926,0.025854722],"genre_scores_gemma":[0.027963495,0.0077763246,0.015754944,0.08652591,0.1366591,0.0003185208,0.12089152,0.011238931,0.5928712],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99626106,0.0003231458,0.000759102,0.00047246472,0.001963785,0.00022035284],"domain_scores_gemma":[0.9810178,0.0038192687,0.0019592887,0.0016112234,0.010626329,0.00096598524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027530564,0.0019103823,0.0011343937,0.0073366184,0.004302847,0.005066941,0.0016080085,0.002408292,0.07453841],"category_scores_gemma":[0.038350426,0.000853998,0.0010176775,0.0060337796,0.001994201,0.003271144,0.0030331006,0.0057369093,0.08304116],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000019850457,0.0000055104333,0.00020253532,0.00004304567,0.0000047941453,0.00004940122,0.000031873107,0.000020020041,0.000044814915,0.00050419837,0.99526817,0.0038057256],"study_design_scores_gemma":[0.00001956898,0.000019506562,0.00249767,0.00026552653,0.000026895012,0.00021107489,0.00016117352,0.00010932777,0.00035738625,0.0012387763,0.9950507,0.000042275773],"about_ca_topic_score_codex":0.03392798,"about_ca_topic_score_gemma":0.03291591,"teacher_disagreement_score":0.07453841,"about_ca_system_score_codex":0.0035472228,"about_ca_system_score_gemma":0.005664972,"threshold_uncertainty_score":0.2493558},"labels":[],"label_agreement":null},{"id":"W4205407960","doi":"10.3847/1538-4357/ac341e","title":"Spatially Resolved Stellar Spectroscopy of the Ultra-diffuse Galaxy Dragonfly 44. III. Evidence for an Unexpected Star Formation History under Conventional Galaxy Evolution Processes","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Galaxy; Population; Physics; Astrophysics","score_opus":0.022917205675475984,"score_gpt":0.24321451301954375,"score_spread":0.22029730734406777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4205407960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99837226,0.00006996078,0.00030674698,0.000026917962,0.000002537534,0.0000024827766,0.00014617835,0.000022268428,0.001050635],"genre_scores_gemma":[0.9983407,0.000033555127,0.00069969747,0.00003257856,0.0000034159932,0.000003498312,0.00028128154,0.0000065864024,0.00059867394],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994326,0.000003387422,0.0000013843119,0.000021073187,0.000013850032,0.000017022416],"domain_scores_gemma":[0.9998765,0.00001269038,0.000025313304,0.0000205897,0.000020714688,0.000044220207],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009131392,0.0001315541,0.00011942046,0.0005045607,0.0002485266,0.00022349924,0.00021443133,0.00022195792,0.0013378316],"category_scores_gemma":[0.0001619187,0.00014502036,0.000113031354,0.00022013213,0.00021251135,0.00016644808,0.0004266469,0.0002355368,0.00022572262],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019095387,0.000083552935,0.6445669,0.000055152275,0.0001041127,0.0004991744,0.00050935993,0.00043521557,0.3306996,0.0005649293,0.001071705,0.021219306],"study_design_scores_gemma":[0.0000052865194,0.00006872243,0.9891466,0.000004108269,0.000025435089,0.00040600623,0.00015307406,0.00046538035,0.007721066,0.000116209856,0.0018810125,0.0000071933414],"about_ca_topic_score_codex":0.002714956,"about_ca_topic_score_gemma":0.007006973,"teacher_disagreement_score":0.002714956,"about_ca_system_score_codex":0.00025985896,"about_ca_system_score_gemma":0.00007158484,"threshold_uncertainty_score":0.0053982735},"labels":[],"label_agreement":null},{"id":"W4205865801","doi":"10.3847/1538-4357/ac3424","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Detection of a Dense SiO Jet in the Evolved Protostellar Phase","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; Agencia Nacional de Investigación y Desarrollo; National Research Foundation of Korea; Chinese Academy of Sciences; Academia Sinica; National Radio Astronomy Observatory; National Natural Science Foundation of China; Natural Sciences and Engineering Research Council of Canada; National Science Council; Science and Technology Facilities Council; National Research Foundation; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Protostar; Physics; Astrophysics; Astronomy; Accretion (finance); Star formation; Submillimeter Array; Outflow; Spectral index; Jet (fluid); Stars; Spectral line","score_opus":0.019996897214926316,"score_gpt":0.26456802345065117,"score_spread":0.24457112623572486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4205865801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99895096,0.000072503186,0.000039254985,0.000013193565,0.0000022191687,0.0000053245344,0.0004326387,0.000013161569,0.00047056703],"genre_scores_gemma":[0.9987929,0.000054827535,0.00014090863,0.000020533127,0.0000057424545,0.0000049780388,0.00070145185,0.0000045976544,0.00027408908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999136,0.0000071409045,0.0000051891125,0.000026229829,0.000021002681,0.000026811933],"domain_scores_gemma":[0.99979764,0.000013092818,0.000072413866,0.000014861144,0.000017850713,0.00008402519],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014629214,0.0002658503,0.00013603154,0.001243034,0.00042323227,0.00033629636,0.00026229135,0.0002004673,0.000869616],"category_scores_gemma":[0.00015567314,0.00012509835,0.0001745347,0.0007563697,0.00019204724,0.00014229422,0.00048721067,0.00012617488,0.00025993277],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009045474,0.00002256388,0.9796847,0.000029256471,0.000038867904,0.0005198088,0.00033074824,0.00005330075,0.014557359,0.000055338824,0.0003969783,0.004220623],"study_design_scores_gemma":[0.0000026672537,0.000017676162,0.99870396,0.0000035507583,0.000007506267,0.00018494762,0.00016375359,0.00006848957,0.00037921616,0.000010930619,0.00045577425,0.0000015608929],"about_ca_topic_score_codex":0.010495274,"about_ca_topic_score_gemma":0.013931401,"teacher_disagreement_score":0.010495274,"about_ca_system_score_codex":0.00025589563,"about_ca_system_score_gemma":0.00018102034,"threshold_uncertainty_score":0.020868361},"labels":[],"label_agreement":null},{"id":"W4205964010","doi":"10.3847/1538-4357/ac3756","title":"X-Ray Burst and Persistent Emission Properties of the Magnetar SGR 1830-0645 in Outburst","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Aeronautics and Space Administration","keywords":"Magnetar; Physics; Materials science; Astrophysics; Analytical Chemistry (journal); Chemistry; Pulsar","score_opus":0.014534213912414743,"score_gpt":0.2561418947996418,"score_spread":0.24160768088722703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4205964010","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99729985,0.00026096465,0.00028505738,0.000026086971,0.000010750342,0.000006724743,0.0007968881,0.00008353788,0.0012300722],"genre_scores_gemma":[0.9967064,0.00007559148,0.00039296199,0.000051133557,0.000015405529,0.000005662995,0.0021725234,0.00003852508,0.00054182333],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999838,0.000013947356,0.0000140682805,0.000055655615,0.000040697127,0.00003767363],"domain_scores_gemma":[0.999551,0.000028883309,0.00014265064,0.00006474841,0.00006914342,0.00014362241],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030633213,0.0002947924,0.0005634242,0.000587841,0.00035259538,0.0007664268,0.00029779517,0.00024505245,0.0009721137],"category_scores_gemma":[0.00041029332,0.0001809658,0.00030101844,0.00045557966,0.00020289872,0.00020923193,0.0006369596,0.0003631716,0.0006945745],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009040715,0.00014855721,0.9066412,0.00010311162,0.00015989183,0.0013776527,0.000571287,0.0007167867,0.0731704,0.0001557184,0.0018821105,0.014169186],"study_design_scores_gemma":[0.000009116318,0.000092826514,0.99618727,0.0000048601814,0.000023091541,0.00029500035,0.00007355959,0.0003420387,0.0015329879,0.00001734048,0.001415716,0.0000063507014],"about_ca_topic_score_codex":0.003669417,"about_ca_topic_score_gemma":0.0056743883,"teacher_disagreement_score":0.003669417,"about_ca_system_score_codex":0.00028455458,"about_ca_system_score_gemma":0.00011352121,"threshold_uncertainty_score":0.0072960854},"labels":[],"label_agreement":null},{"id":"W4206481302","doi":"10.3847/1538-4357/ac4502","title":"Let the Great World Spin: Revealing the Stormy, Turbulent Nature of Young Giant Exoplanet Analogs with the Spitzer Space Telescope","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":83,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Brown dwarf; Exoplanet; Physics; Astrophysics; Angular momentum; Rotation period; Astronomy; Stellar classification; Amplitude; Spitzer Space Telescope; Low Mass; Rotation (mathematics); Planet; Telescope; Stars; Geometry","score_opus":0.007214615903392919,"score_gpt":0.21291655004638566,"score_spread":0.20570193414299273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4206481302","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988372,0.000057281795,0.00021595566,0.00002525241,0.0000023291325,0.0000022240915,0.00023680729,0.000021151922,0.0006018501],"genre_scores_gemma":[0.9990515,0.00003628158,0.00034335416,0.00001912472,0.000008851859,0.000002645934,0.00035773785,0.0000090332915,0.00017145046],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999418,0.000005822396,0.0000033296692,0.000015391815,0.00001604654,0.000017553699],"domain_scores_gemma":[0.99963605,0.00003740214,0.00013710157,0.000037442256,0.00004252526,0.000109427056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024423117,0.00013857785,0.00012475373,0.0010665221,0.0002966512,0.00036287034,0.00016158046,0.00015201404,0.0007544819],"category_scores_gemma":[0.0004075558,0.00009488014,0.00014490451,0.00062362483,0.00023541374,0.00031739468,0.00040893134,0.00017992109,0.00025131038],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008006843,0.000021941889,0.97426426,0.000012990534,0.000039476872,0.00033183486,0.0005127635,0.00016244556,0.018156642,0.000103492894,0.00055055687,0.005763498],"study_design_scores_gemma":[0.000001045934,0.000009924767,0.99922514,0.0000013019417,0.0000034969664,0.000091676106,0.00011154837,0.00013138511,0.00019844709,0.000027207545,0.00019723183,0.0000016731108],"about_ca_topic_score_codex":0.001959288,"about_ca_topic_score_gemma":0.0055893203,"teacher_disagreement_score":0.001959288,"about_ca_system_score_codex":0.00018401499,"about_ca_system_score_gemma":0.000087986715,"threshold_uncertainty_score":0.0038957},"labels":[],"label_agreement":null},{"id":"W4206614000","doi":"10.3847/1538-4357/ac3980","title":"The Effects of Metallicity on Convective Overshoot Behavior in Models of δ Scuti Variable Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Mount Allison University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Metallicity; Physics; Stars; Astrophysics; Overshoot (microwave communication); Convection; Effective temperature; Star (game theory); Thermodynamics; Computer science","score_opus":0.010058542471077197,"score_gpt":0.22122510284905852,"score_spread":0.21116656037798132,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4206614000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978029,0.000039102473,0.0008055804,0.00007867694,0.000004693915,0.000006006735,0.00015687029,0.000063571286,0.0010426884],"genre_scores_gemma":[0.99901605,0.00002396248,0.00060643646,0.00001406814,0.000002498715,0.000008670792,0.000113769245,0.000024277635,0.00019035219],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998685,0.000053311203,0.00001100036,0.00002609626,0.000014342332,0.000026833695],"domain_scores_gemma":[0.9989779,0.0005970356,0.00013861021,0.0001043443,0.000084219566,0.00009794764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005957658,0.00047610773,0.0004113647,0.0005210983,0.000537047,0.0009067942,0.00075590255,0.0004838311,0.0009601201],"category_scores_gemma":[0.0019433202,0.00028917714,0.00062083814,0.00032754714,0.000579472,0.00048608557,0.00059479644,0.00040763026,0.00012367069],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016868376,0.00008070844,0.052304998,0.000024478068,0.00006523708,0.0001164024,0.00013876846,0.9416241,0.0025040647,0.0008874983,0.00036544848,0.001719628],"study_design_scores_gemma":[0.000031659776,0.000037434806,0.0059571215,0.0000059156623,0.000017441822,0.000016632599,0.000038938106,0.99262553,0.000800921,0.0002974548,0.00016276298,0.000008114187],"about_ca_topic_score_codex":0.021415826,"about_ca_topic_score_gemma":0.009493238,"teacher_disagreement_score":0.021415826,"about_ca_system_score_codex":0.0010002261,"about_ca_system_score_gemma":0.00038039748,"threshold_uncertainty_score":0.042582333},"labels":[],"label_agreement":null},{"id":"W4206890056","doi":"10.3847/1538-4357/ac4254","title":"Exploring the S-process History in the Galactic Disk: Cerium Abundances and Gradients in Open Clusters from the OCCAM/APOGEE Sample","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Science and Technology Facilities Council; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"occam; Sample (material); Cerium; Process (computing); Disc; Cusp (singularity); Occam's razor; Astrophysics; Physics; Computer science; Materials science; Galaxy formation and evolution; Galaxy; Mathematics; Geometry; Statistics; Operating system; Metallurgy","score_opus":0.05059034785730505,"score_gpt":0.25056240164834237,"score_spread":0.19997205379103733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4206890056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99948174,0.0000686794,0.000032121254,0.000007646183,6.767424e-7,0.0000013297278,0.0002160569,0.0000028372042,0.0001888719],"genre_scores_gemma":[0.9988182,0.00006132098,0.00009380155,0.0000062521212,0.0000029301705,0.0000031553882,0.0007760508,0.0000067751416,0.00023146732],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998573,0.0000149776815,0.000008105306,0.00006128042,0.000021670536,0.00003665676],"domain_scores_gemma":[0.9995041,0.00007034662,0.00014076699,0.00006257176,0.00008280246,0.00013944048],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024242298,0.0002972715,0.00029331804,0.0021892188,0.00044670736,0.0007525313,0.00034639478,0.00023026003,0.001244067],"category_scores_gemma":[0.00070451206,0.00014904611,0.00021304634,0.0013369145,0.00036234714,0.00032782578,0.001116102,0.0001510598,0.00043820552],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021742757,0.00001992342,0.98941493,0.000017272598,0.000066356195,0.00011672628,0.0005267451,0.00013743358,0.0040266323,0.00005392185,0.00018426178,0.005218436],"study_design_scores_gemma":[0.0000021396572,0.000010365297,0.9990963,0.0000022332329,0.000008365863,0.00006314045,0.00023513727,0.00008995085,0.00018279774,0.000013294463,0.00029406932,0.0000022601955],"about_ca_topic_score_codex":0.012094584,"about_ca_topic_score_gemma":0.016915856,"teacher_disagreement_score":0.012094584,"about_ca_system_score_codex":0.00036015527,"about_ca_system_score_gemma":0.00014324977,"threshold_uncertainty_score":0.024048388},"labels":[],"label_agreement":null},{"id":"W4210264104","doi":"10.3847/1538-4357/ac313f","title":"Extremely Broad Lyα Line Emission from the Molecular Intragroup Medium in Stephan’s Quintet: Evidence for a Turbulent Cascade in a Highly Clumpy Multiphase Medium?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Fluid Dynamics and Turbulent Flows","field":"Engineering","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Institut Universitaire de France; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Max-Planck-Gesellschaft; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Cascade; Turbulence; Line (geometry); Astrophysics; Physics; Mechanics; Chemistry; Chromatography; Geometry","score_opus":0.017518581400209916,"score_gpt":0.2500154996846379,"score_spread":0.23249691828442795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210264104","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997445,0.0000082277,0.00003201704,0.0000093258905,5.78394e-7,9.600565e-7,0.000010110443,0.0000018694592,0.00019243633],"genre_scores_gemma":[0.99987495,0.0000032041303,0.000039432736,0.0000049766118,9.3806534e-7,6.298359e-7,0.000013425068,8.9177837e-7,0.00006159174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999598,0.0000025420154,9.675547e-7,0.000010936258,0.0000103262255,0.000015354663],"domain_scores_gemma":[0.99985456,0.000011586059,0.00003649944,0.000007343311,0.000019012547,0.00007099664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000060011185,0.00015851948,0.0001507957,0.0004397375,0.0007078335,0.00036712168,0.0003524344,0.00021383473,0.0015529756],"category_scores_gemma":[0.0001355783,0.00013659813,0.0001058139,0.00023735515,0.00040501374,0.00020067478,0.0006526324,0.00023104867,0.00014653213],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035980504,0.000110982655,0.71892637,0.000026801461,0.000052782383,0.0068143867,0.0026470681,0.0005043216,0.26335537,0.0003355294,0.00025497214,0.0066115763],"study_design_scores_gemma":[0.000009413698,0.000110382345,0.990666,0.00000387185,0.000014421601,0.0011824332,0.0014967027,0.0012728743,0.004425399,0.00013192366,0.0006738409,0.000012612546],"about_ca_topic_score_codex":0.0072099958,"about_ca_topic_score_gemma":0.014045074,"teacher_disagreement_score":0.0072099958,"about_ca_system_score_codex":0.00027779516,"about_ca_system_score_gemma":0.0001215784,"threshold_uncertainty_score":0.01433605},"labels":[],"label_agreement":null},{"id":"W4210379579","doi":"10.3847/1538-4357/abfafe","title":"The NANOGrav 12.5 Year Data Set: Monitoring Interstellar Scattering Delays","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"National Science Foundation","keywords":"Physics; Astronomy; Scattering; Interstellar medium; Astrophysics; Galaxy; Optics","score_opus":0.03168209256886966,"score_gpt":0.2598843479966677,"score_spread":0.22820225542779804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210379579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9267254,0.00028844853,0.0026763042,0.00013651773,0.000049585862,0.00005851397,0.06292807,0.0005873097,0.0065498115],"genre_scores_gemma":[0.8268248,0.00018521909,0.007916773,0.00011224575,0.00005691903,0.00012485881,0.16217995,0.00017179963,0.0024274846],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997173,0.000031842606,0.0000258843,0.00007276392,0.00012450937,0.000027736425],"domain_scores_gemma":[0.9990428,0.00010590009,0.00023662171,0.00023426051,0.00028479894,0.00009565643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006889757,0.00033611414,0.00036595456,0.0018232021,0.00029985153,0.0005760986,0.00044943622,0.00034541963,0.0009898324],"category_scores_gemma":[0.0011272491,0.0001834934,0.00025018794,0.0020319636,0.00015180313,0.00043033942,0.00046448788,0.0003290802,0.0008839799],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013649917,0.00026392567,0.8337311,0.000267024,0.0003316117,0.00048657888,0.0004357526,0.013547879,0.04672759,0.0013305492,0.02822176,0.07329128],"study_design_scores_gemma":[0.00008034208,0.00016440221,0.940151,0.00002984027,0.000066804016,0.00023907791,0.00011690572,0.018590238,0.012163724,0.00037989637,0.02796822,0.00004956652],"about_ca_topic_score_codex":0.007921193,"about_ca_topic_score_gemma":0.015444326,"teacher_disagreement_score":0.007921193,"about_ca_system_score_codex":0.00030853716,"about_ca_system_score_gemma":0.00029926578,"threshold_uncertainty_score":0.01575017},"labels":[],"label_agreement":null},{"id":"W4210506696","doi":"10.3847/1538-4357/ac3a69","title":"Metallicity in Quasar Broad-line Regions at Redshift ∼ 6","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Natural Science Foundation of China; National Key Research and Development Program of China; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Quasar; Astrophysics; Redshift; Metallicity; Astronomy; Emission spectrum; Photoionization; Spectral line; Galaxy; Ionization","score_opus":0.013320540974657485,"score_gpt":0.2283917421898674,"score_spread":0.21507120121520992,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210506696","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99964356,0.000048051403,0.00002054701,0.000005604297,6.0671687e-7,8.214933e-7,0.0001147617,0.0000036871377,0.00016239933],"genre_scores_gemma":[0.9996817,0.00001691804,0.000024200277,0.000003805421,0.0000019266847,5.009978e-7,0.00017629053,0.0000015596579,0.000093229006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998629,0.000016436714,0.000008943598,0.000036433565,0.000025521615,0.000049812792],"domain_scores_gemma":[0.9991787,0.000075898024,0.00047909733,0.00003790577,0.00005652459,0.00017185851],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024993857,0.00017720295,0.00018142987,0.0017087774,0.00022339592,0.00053529587,0.00018351508,0.00023983202,0.0015704624],"category_scores_gemma":[0.0006288709,0.0001144896,0.00016545404,0.0006507678,0.0002548951,0.00027005066,0.00035647565,0.00019890812,0.00039871963],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004078844,0.000012434244,0.9961443,0.000003202448,0.00001454279,0.00004563055,0.000106886866,0.00003177861,0.0025452462,0.000030405257,0.000033015294,0.0009916844],"study_design_scores_gemma":[4.881578e-7,0.000010209019,0.99976164,5.7396085e-7,0.0000019833901,0.000041886884,0.000032141892,0.000024635608,0.00008208071,0.0000070522046,0.000036817524,4.7738064e-7],"about_ca_topic_score_codex":0.0023433017,"about_ca_topic_score_gemma":0.0026694415,"teacher_disagreement_score":0.0023433017,"about_ca_system_score_codex":0.0001407452,"about_ca_system_score_gemma":0.00004945277,"threshold_uncertainty_score":0.005253732},"labels":[],"label_agreement":null},{"id":"W4210608581","doi":"10.3847/1538-4357/ac397d","title":"A Study of the Stochastic Photometric Variability in the Winds of Galactic Wolf–Rayet Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Stars; Astrophysics; Wolf–Rayet star; Astronomy","score_opus":0.014538752318464144,"score_gpt":0.2406447276985411,"score_spread":0.22610597538007696,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210608581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99940217,0.000020919057,0.0003743421,0.000004529321,7.5526924e-7,0.0000015531251,0.0001039055,0.0000047973667,0.000087052584],"genre_scores_gemma":[0.9994236,0.000013053206,0.00015789749,0.0000012854763,0.0000027069566,0.0000015364213,0.0003623756,0.0000023787234,0.000035195255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980515,0.00005138845,0.000017582122,0.00005103953,0.00004668016,0.000028136588],"domain_scores_gemma":[0.99874485,0.00049713143,0.00037594922,0.00010805268,0.00014731631,0.000126697],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004987966,0.0001477756,0.00017346838,0.0011181042,0.00020629851,0.0003592075,0.0001394611,0.00020069067,0.00032980228],"category_scores_gemma":[0.00224558,0.00011702799,0.00024446624,0.00082714105,0.00016792984,0.00021906178,0.00022478834,0.00014952983,0.00010910188],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010570086,0.00002810863,0.9835442,0.0000106823445,0.00007031626,0.00011055287,0.00010556234,0.0025992617,0.008262638,0.00012377404,0.000054494216,0.004984741],"study_design_scores_gemma":[0.000002153162,0.000037670554,0.99326926,0.0000017170056,0.000008746408,0.00010150778,0.000041634084,0.005816751,0.0005262407,0.000059779406,0.00013033062,0.000004181356],"about_ca_topic_score_codex":0.0020978693,"about_ca_topic_score_gemma":0.0019049032,"teacher_disagreement_score":0.0020978693,"about_ca_system_score_codex":0.00017542363,"about_ca_system_score_gemma":0.00010106206,"threshold_uncertainty_score":0.0041712523},"labels":[],"label_agreement":null},{"id":"W4210637903","doi":"10.3847/1538-4357/ac3a6b","title":"Variational Image Feature Extraction for the Event Horizon Telescope","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Very-long-baseline interferometry; Feature (linguistics); Telescope; Image (mathematics); Orientation (vector space); Physics; Event (particle physics); Artificial intelligence; Computer science; Horizon; Feature detection (computer vision); Domain (mathematical analysis); Computer vision; Image processing; Astrophysics; Mathematics; Astronomy; Geometry; Mathematical analysis","score_opus":0.010504449730239453,"score_gpt":0.25333289951370763,"score_spread":0.24282844978346818,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210637903","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07484908,0.00014586475,0.92324483,0.00014799827,0.000012841443,0.0000261371,0.00032833632,0.00061663,0.0006283718],"genre_scores_gemma":[0.51402336,0.00012054558,0.4831979,0.000050924544,0.000022930126,0.000036312726,0.0013202871,0.00019289233,0.0010349108],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997408,0.000063323896,0.000011528554,0.000059029997,0.00008559034,0.00003971391],"domain_scores_gemma":[0.999468,0.0002430863,0.00007179863,0.00008596671,0.000098579185,0.000032523996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009849586,0.00042383932,0.00053207227,0.000928254,0.00028333798,0.0007396667,0.00084337336,0.0006291667,0.0010340529],"category_scores_gemma":[0.0022300675,0.00036957551,0.00080026046,0.00066857296,0.00047647973,0.0007338962,0.0006803371,0.00083831645,0.00028549152],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025727283,0.00011594769,0.0065569635,0.00012835562,0.0001757689,0.00015324901,0.00013692016,0.64586586,0.06710685,0.027103836,0.0027639645,0.24963497],"study_design_scores_gemma":[0.0000028185893,0.000006740095,0.0007827261,0.0000014014588,0.0000027832714,0.00001676798,0.000006709658,0.9941028,0.0020155925,0.0027108528,0.00034533537,0.0000054966795],"about_ca_topic_score_codex":0.007389886,"about_ca_topic_score_gemma":0.0069194078,"teacher_disagreement_score":0.007389886,"about_ca_system_score_codex":0.0006373479,"about_ca_system_score_gemma":0.0006883092,"threshold_uncertainty_score":0.014693737},"labels":[],"label_agreement":null},{"id":"W4210714783","doi":"10.3847/1538-4357/ac382f","title":"Molecular Gas Properties and CO-to-H<sub>2</sub> Conversion Factors in the Central Kiloparsec of NGC 3351","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; National Astronomical Observatory of Japan; Ministerio de Ciencia e Innovación; European Commission; Associated Universities; Agencia Estatal de Investigación; National Radio Astronomy Observatory; Ministerio de Ciencia, Innovación y Universidades; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Natural Sciences and Engineering Research Council of Canada; National Science Council; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; Carbon monoxide; Chemistry; Catalysis","score_opus":0.013330635465541798,"score_gpt":0.2090744051394823,"score_spread":0.1957437696739405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210714783","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994814,0.000038560192,0.00009946981,0.000008174969,4.901983e-7,0.0000012699047,0.00017732073,0.000016525091,0.00017686676],"genre_scores_gemma":[0.99954164,0.000015731119,0.000118404976,0.000003831769,0.0000015316825,0.0000014838046,0.0002589181,0.0000030351678,0.000055370012],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994934,0.000003947207,0.0000023072082,0.000018020302,0.000013147412,0.000013304369],"domain_scores_gemma":[0.9997402,0.000040833642,0.00010269444,0.000018426783,0.000032943695,0.00006495216],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010304561,0.00016873125,0.00015564213,0.00058207894,0.0003116567,0.0003402308,0.0002182094,0.0001910247,0.0008418478],"category_scores_gemma":[0.00022997745,0.00015925153,0.00021306523,0.00032024577,0.00016332432,0.00016381874,0.00020489316,0.00020896179,0.00019571929],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023077386,0.00005385413,0.92427826,0.000026239275,0.00007413055,0.00031142632,0.0002795596,0.0026836148,0.06629751,0.0001309194,0.0002616258,0.0053721634],"study_design_scores_gemma":[0.0000014087545,0.0000080741,0.99804556,0.0000011509394,0.000006943159,0.000043588818,0.00003425269,0.0011686502,0.00060190895,0.000010333109,0.000076103584,0.0000019833344],"about_ca_topic_score_codex":0.023081033,"about_ca_topic_score_gemma":0.019633768,"teacher_disagreement_score":0.023081033,"about_ca_system_score_codex":0.0003948072,"about_ca_system_score_gemma":0.00006697744,"threshold_uncertainty_score":0.04589337},"labels":[],"label_agreement":null},{"id":"W4210824600","doi":"10.3847/1538-4357/ac3fb7","title":"The Fast Evolving, Tremendous Blue Superoutburst in ASASSN-21au Reveals a Dichotomy in the Outbursts of Long-period AM CVns","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Stockholms Universitet; California Institute of Technology; European Space Agency; University of Washington; University of Alberta; National Science Foundation","keywords":"Astrophysics; Physics; White dwarf; Light curve; Dwarf nova; Brightness; Amplitude; Accretion (finance); Astronomy; Stars; Optics","score_opus":0.01252154773653123,"score_gpt":0.24020281676963479,"score_spread":0.22768126903310357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210824600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995981,0.000024871424,0.000037010494,0.0000061137266,0.0000020793807,0.000001200498,0.000030662446,0.0000033943131,0.0002965515],"genre_scores_gemma":[0.9997085,0.000007881896,0.000041615498,0.000005502833,0.000002687743,0.0000018713897,0.00010024262,0.0000018700873,0.00012981903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999938,0.000005391305,0.0000038590706,0.000021941201,0.000014411791,0.000016356902],"domain_scores_gemma":[0.9997267,0.000025720587,0.000051074378,0.0000213838,0.00004773776,0.00012731065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011258525,0.0001244942,0.00025082566,0.0005145687,0.00044050338,0.00038301016,0.0001962354,0.00020624504,0.0006196189],"category_scores_gemma":[0.00027380494,0.00009566446,0.00014938589,0.000249914,0.00022482799,0.00013708562,0.00044970278,0.00025836137,0.00012279736],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044259982,0.0000729411,0.84812313,0.000025804446,0.00004053887,0.0016070036,0.0008401789,0.00033552776,0.1394705,0.00024056253,0.00031285186,0.008488391],"study_design_scores_gemma":[0.0000021823641,0.000030915275,0.99820983,0.000001998792,0.0000038540215,0.00027487217,0.00013633762,0.00036645902,0.00076182274,0.000035442343,0.00017297146,0.0000031933628],"about_ca_topic_score_codex":0.0033036184,"about_ca_topic_score_gemma":0.0071295626,"teacher_disagreement_score":0.0033036184,"about_ca_system_score_codex":0.00028242372,"about_ca_system_score_gemma":0.00009619502,"threshold_uncertainty_score":0.0065687895},"labels":[],"label_agreement":null},{"id":"W4210872909","doi":"10.3847/1538-4357/ac469b","title":"Powering Stellar Magnetism: Energy Transfers in Cyclic Dynamos of Sun-like Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":80,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"","keywords":"Physics; Algorithm; Computer science","score_opus":0.004351574999047064,"score_gpt":0.196364905573175,"score_spread":0.19201333057412795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210872909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950759,0.000039889303,0.0024611808,0.00008963768,0.000007987506,0.0000068595295,0.00012156917,0.000083822786,0.0021132284],"genre_scores_gemma":[0.99936277,0.000013341873,0.0003681291,0.000013871262,0.000002572612,0.000004338384,0.00004409241,0.00001980791,0.0001710485],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994767,0.000014218212,0.0000032792545,0.000010606947,0.000011044732,0.000013126067],"domain_scores_gemma":[0.999721,0.00010909373,0.000051438547,0.0000361254,0.000031361546,0.000050985418],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022042554,0.00021366047,0.00024439773,0.00024155891,0.0003176096,0.00048213408,0.00041763374,0.00034471907,0.0018477205],"category_scores_gemma":[0.001005549,0.00015303791,0.00036689528,0.00024195376,0.00047285963,0.00041198946,0.0005050453,0.00028895828,0.00013679978],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023556339,0.000117515825,0.033185784,0.000050828217,0.00008581717,0.00025208064,0.00015873589,0.9441044,0.010319512,0.005701409,0.0006903865,0.005098014],"study_design_scores_gemma":[0.000052862204,0.00004340835,0.008683661,0.0000038600506,0.000011290812,0.00003597052,0.000042595762,0.98535144,0.0017643628,0.003640861,0.00035685915,0.000012816295],"about_ca_topic_score_codex":0.004783707,"about_ca_topic_score_gemma":0.0025640128,"teacher_disagreement_score":0.004783707,"about_ca_system_score_codex":0.0005043809,"about_ca_system_score_gemma":0.0002923523,"threshold_uncertainty_score":0.009511769},"labels":[],"label_agreement":null},{"id":"W4210960386","doi":"10.3847/1538-4357/ac3b55","title":"Subgalactic Scaling Relations with T <sub>e</sub>-based Metallicities of Low-metallicity Regions in Galaxies: Metal-poor Gas Inflow May Have Important Effects?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Metallicity; Astrophysics; Galaxy; Scaling; Star formation; Elliptical galaxy; Stars; Astronomy; Geometry","score_opus":0.006257026881728448,"score_gpt":0.1990307645345927,"score_spread":0.19277373765286426,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210960386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864835,0.00006558051,0.00016047616,0.00005087023,0.0000023148689,0.0000014957195,0.00018570504,0.000009598818,0.0008756798],"genre_scores_gemma":[0.9996606,0.0000136968165,0.00004212291,0.000009484702,0.0000043803298,8.4815395e-7,0.00014378576,0.0000041647077,0.00012086355],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998374,0.000026325964,0.000013679525,0.00006054651,0.000023281731,0.000038803202],"domain_scores_gemma":[0.9968911,0.00069539895,0.0011694812,0.00033122188,0.00026130464,0.00065151794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034448795,0.0001757253,0.00020409141,0.0013973676,0.00026525307,0.0009704243,0.00023196492,0.00030114618,0.0041567157],"category_scores_gemma":[0.0027035433,0.00011343507,0.00019624775,0.0010613009,0.00059671793,0.000624049,0.0004617172,0.00029864698,0.0007678223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000021798896,0.000007949556,0.9969311,0.0000028476209,0.000017462666,0.000028237244,0.00009766765,0.00007668061,0.001117194,0.00016361247,0.00009887916,0.0014365329],"study_design_scores_gemma":[9.725188e-7,0.0000051677953,0.99920577,0.0000012583372,0.000003567889,0.000020626007,0.00009252242,0.00029458746,0.00009459422,0.00017607506,0.000103918275,0.0000010379406],"about_ca_topic_score_codex":0.0032084268,"about_ca_topic_score_gemma":0.0033902004,"teacher_disagreement_score":0.0041567157,"about_ca_system_score_codex":0.00024194916,"about_ca_system_score_gemma":0.0000801343,"threshold_uncertainty_score":0.013905585},"labels":[],"label_agreement":null},{"id":"W4210985836","doi":"10.3847/1538-4357/ac4156","title":"Using Computational Models to Uncover the Parameters of Three Kepler Binaries: KIC 5957123, KIC 8314879, and KIC 10727668*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Mount Allison University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Kepler; Astrophysics; Astronomy; Stars","score_opus":0.043542252581398495,"score_gpt":0.24647134080917918,"score_spread":0.2029290882277807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4210985836","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9857831,0.000040320287,0.011832712,0.00012796615,0.000004976169,0.000024894562,0.0002866239,0.00010782862,0.0017916763],"genre_scores_gemma":[0.9919275,0.00002960104,0.0072217467,0.00002078917,0.0000042234915,0.000038200866,0.00034178322,0.00003053765,0.00038564275],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988854,0.000040040162,0.00000654443,0.000028064378,0.000016614627,0.000020196207],"domain_scores_gemma":[0.99788135,0.0017189507,0.00012989428,0.00008594926,0.000103374354,0.00008042431],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00091275113,0.00048763066,0.0005398801,0.00087043084,0.0009894044,0.001191902,0.00086209626,0.0007125275,0.0018586842],"category_scores_gemma":[0.004095378,0.0006131308,0.0006392517,0.00064288947,0.00050938805,0.00075139303,0.00058425637,0.0008609236,0.00018459807],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049574726,0.000028484747,0.008530317,0.000009664929,0.000024724128,0.00002840632,0.00003473694,0.98767495,0.00024631975,0.001642984,0.00006786797,0.0016618897],"study_design_scores_gemma":[0.000009036074,0.000005517739,0.00074969395,0.000001912489,0.0000057139623,0.0000038804114,0.000012634061,0.99825984,0.00013213925,0.0007692362,0.00004757725,0.0000028320444],"about_ca_topic_score_codex":0.04614255,"about_ca_topic_score_gemma":0.043756545,"teacher_disagreement_score":0.04614255,"about_ca_system_score_codex":0.0024897463,"about_ca_system_score_gemma":0.0018409202,"threshold_uncertainty_score":0.09174794},"labels":[],"label_agreement":null},{"id":"W4212801530","doi":"10.3847/1538-4357/ac4d2a","title":"The Global Dynamical Atlas of the Milky Way Mergers: Constraints from Gaia EDR3–based Orbits of Globular Clusters, Stellar Streams, and Satellite Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":163,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Office of Science; Max-Planck-Institut für Astronomie; National Development and Reform Commission; Ministerio de Ciencia e Innovación; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; Agence Nationale de la Recherche; Ministerio de Ciencia, Innovación y Universidades; York University; Gruber Foundation; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Institut sur la Nutrition et les Aliments Fonctionnels; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Agencia Estatal de Investigación; Yale University; Vanderbilt University; University of Arizona; Alexander von Humboldt-Stiftung; National Science Foundation; U.S. Department of Energy","keywords":"Physics; Globular cluster; Milky Way; Astronomy; Galaxy; Satellite; Satellite galaxy; Astrophysics; Star cluster; Atlas (anatomy); Galactic astronomy; Stellar dynamics; Medicine","score_opus":0.006671869966778122,"score_gpt":0.2082249909614791,"score_spread":0.20155312099470096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212801530","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972019,0.00007567076,0.00053911685,0.000014804195,0.0000011163581,0.00000586974,0.0010260725,0.000056185327,0.0010792235],"genre_scores_gemma":[0.99669504,0.000034973134,0.0011779767,0.000008104381,0.0000028744244,0.000005792056,0.0019225818,0.00001889405,0.00013378882],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998492,0.000020897578,0.000013202557,0.000054926622,0.000030396463,0.000031331638],"domain_scores_gemma":[0.99957556,0.0000497252,0.00018425938,0.00006588976,0.000052029973,0.0000724795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030022138,0.00020515588,0.00015426039,0.0020304653,0.00024422046,0.0005302355,0.00017596288,0.00017209009,0.0006894673],"category_scores_gemma":[0.0005699622,0.00013782196,0.00025223146,0.001269796,0.00024593747,0.00023341655,0.00074569316,0.00011371795,0.00022928274],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000102170205,0.00001771893,0.9714237,0.00002380898,0.0000671748,0.00010688788,0.00025693254,0.0013309531,0.015360656,0.00024884028,0.00047404552,0.010587114],"study_design_scores_gemma":[0.000004867729,0.000010679413,0.9957486,0.0000045465003,0.000018167108,0.00005367276,0.00010583979,0.0020906075,0.0010187428,0.000062679006,0.000878109,0.0000035178969],"about_ca_topic_score_codex":0.0068512233,"about_ca_topic_score_gemma":0.015144854,"teacher_disagreement_score":0.0068512233,"about_ca_system_score_codex":0.0003033616,"about_ca_system_score_gemma":0.00019461189,"threshold_uncertainty_score":0.013622701},"labels":[],"label_agreement":null},{"id":"W4212835244","doi":"10.3847/1538-4357/ac449b","title":"Fast, Slow, Early, Late: Quenching Massive Galaxies at z ∼ 0.8","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":164,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Ulsan National Institute of Science and Technology; Flatiron Health; Simons Foundation; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Star formation; Stellar mass; Metallicity; Photometry (optics); Galaxy formation and evolution; Spectroscopy; Astronomy; Stars","score_opus":0.006225929306915713,"score_gpt":0.2007790595471181,"score_spread":0.1945531302402024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212835244","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999616,0.000029529712,0.000055148565,0.0000064016203,2.3194676e-7,8.824178e-7,0.00017010314,0.0000053908743,0.000116293355],"genre_scores_gemma":[0.999585,0.000008503774,0.00003963489,0.0000021470212,0.0000010393688,7.058026e-7,0.0002867172,0.0000015159362,0.0000747121],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987984,0.00001798084,0.000005814682,0.00004126849,0.000017461216,0.000037626232],"domain_scores_gemma":[0.9992017,0.0001629697,0.00030636333,0.00006864949,0.00006736967,0.000192935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045743713,0.00013651921,0.00015674483,0.0007910987,0.00016423008,0.00052954454,0.00027147692,0.00020301249,0.0011574936],"category_scores_gemma":[0.0010683674,0.000113721966,0.0001749764,0.00035395756,0.00024398004,0.00036036133,0.00043544933,0.00011390951,0.0003436135],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000517723,0.000009768548,0.99623716,0.000003414662,0.000012150223,0.000019572406,0.00009540526,0.0002724801,0.0011579398,0.00011438591,0.00006982875,0.0019561772],"study_design_scores_gemma":[0.0000021206542,0.000017099002,0.99872357,9.3984e-7,0.00000491384,0.00003526925,0.000054494187,0.0008123099,0.00016045994,0.00006512652,0.00012211119,0.0000014330972],"about_ca_topic_score_codex":0.0022147864,"about_ca_topic_score_gemma":0.0024239307,"teacher_disagreement_score":0.0022147864,"about_ca_system_score_codex":0.00017287626,"about_ca_system_score_gemma":0.00006627954,"threshold_uncertainty_score":0.00440377},"labels":[],"label_agreement":null},{"id":"W4212942031","doi":"10.3847/1538-4357/ac43bd","title":"Variable Stars in the Giant Satellite Galaxy Antlia 2","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Lawrence Berkeley National Laboratory; SLAC National Accelerator Laboratory; Fermilab; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; University of Sussex; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University College London; Deutsche Forschungsgemeinschaft; University of Portsmouth; Ohio State University; Institut de Física d'Altes Energies; University of Pennsylvania; National Science Foundation","keywords":"RR Lyrae variable; Physics; Astrophysics; Astronomy; Cepheid variable; Galaxy; Local Group; Stars; Dwarf galaxy; Satellite galaxy; Variable star; Globular cluster","score_opus":0.010299375341010046,"score_gpt":0.2155404960929225,"score_spread":0.20524112075191245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212942031","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991683,0.00007311959,0.000034864133,0.000009370283,0.0000016973986,0.00000275715,0.000109843524,0.000008450536,0.00059157045],"genre_scores_gemma":[0.9989858,0.00005313634,0.00020370289,0.000012370289,0.0000053250806,0.000003129149,0.00055013265,0.0000025955712,0.00018369636],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983525,0.000016552602,0.000012730888,0.000049436174,0.00005126811,0.000034686564],"domain_scores_gemma":[0.99950325,0.000041771396,0.00023585191,0.00004002806,0.00006160614,0.00011749561],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011452083,0.00020053668,0.0001894618,0.0018171507,0.00028968957,0.00052048103,0.00027239913,0.00017541125,0.00060005946],"category_scores_gemma":[0.00048706884,0.00015252395,0.00013059148,0.0009508282,0.00017808832,0.00020186229,0.00059543346,0.00012897502,0.00020120971],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009701607,0.000022746937,0.9824744,0.00001673477,0.000028233637,0.00031584324,0.00035258976,0.00014981598,0.010858489,0.00008841648,0.00032093638,0.005274861],"study_design_scores_gemma":[0.0000032557987,0.000031382384,0.99802774,0.0000028815195,0.0000068009117,0.00028841454,0.00010103902,0.00022273029,0.0002544021,0.000024064211,0.0010353057,0.0000019151137],"about_ca_topic_score_codex":0.008262083,"about_ca_topic_score_gemma":0.012872131,"teacher_disagreement_score":0.008262083,"about_ca_system_score_codex":0.00033505994,"about_ca_system_score_gemma":0.00013460779,"threshold_uncertainty_score":0.016427994},"labels":[],"label_agreement":null},{"id":"W4212968910","doi":"10.3847/1538-4357/ac4418","title":"Hubble Space Telescope Observations of NGC 253 Dwarf Satellites: Three Ultra-faint Dwarf Galaxies*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Physics; Dwarf galaxy; Astrophysics; Astronomy; Local Group; Galaxy; Dwarf spheroidal galaxy; Spiral galaxy; Dwarf galaxy problem; Satellite galaxy; Red-giant branch; Luminosity; Luminosity function; Advanced Camera for Surveys; Hubble space telescope; Globular cluster; Interacting galaxy","score_opus":0.015958862978220363,"score_gpt":0.21816282786655153,"score_spread":0.20220396488833117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212968910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843234,0.00007970427,0.0001430821,0.00001937514,0.0000027254582,0.0000044061835,0.00021084624,0.00002186777,0.0010855505],"genre_scores_gemma":[0.9991543,0.000030266989,0.0002514071,0.000013620768,0.000004107469,0.000002346959,0.00032048274,0.0000020380971,0.00022152408],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999343,0.0000034347029,0.0000042205606,0.000018867786,0.000022212103,0.00001700748],"domain_scores_gemma":[0.99969566,0.000017082397,0.000069534086,0.000026727494,0.000037735543,0.0001533449],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001281589,0.00019699053,0.00019498708,0.00057865045,0.00047388166,0.00038627177,0.00021316216,0.00027347516,0.0008649255],"category_scores_gemma":[0.00017045489,0.00010038886,0.00018686379,0.00036019133,0.00028403933,0.00014040753,0.0002721951,0.00019197784,0.00030833867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017874375,0.0001056914,0.93096393,0.000026660655,0.00005801781,0.0012293439,0.00058484793,0.00042721984,0.054516796,0.00037227507,0.0008082929,0.010728206],"study_design_scores_gemma":[0.000008409166,0.000046808815,0.9961361,0.0000040079663,0.000014162908,0.00044456395,0.00011302628,0.00027774952,0.0019097357,0.00005517283,0.0009841505,0.000006083716],"about_ca_topic_score_codex":0.011475356,"about_ca_topic_score_gemma":0.024449399,"teacher_disagreement_score":0.011475356,"about_ca_system_score_codex":0.00065174076,"about_ca_system_score_gemma":0.00018287072,"threshold_uncertainty_score":0.022817135},"labels":[],"label_agreement":null},{"id":"W4212972699","doi":"10.3847/1538-4357/ac4045","title":"The NANOGrav 12.5 yr Data Set: Polarimetry and Faraday Rotation Measures from Observations of Millisecond Pulsars with the Green Bank Telescope","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geophysics and Sensor Technology","field":"Engineering","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"Office of Naval Research; West Virginia Space Grant Consortium; National Aeronautics and Space Administration; Science and Technology Facilities Council; National Science Foundation","keywords":"Polarimetry; Faraday effect; Green Bank Telescope; Millisecond pulsar; Physics; Pulsar; Astronomy; Telescope; Rotation (mathematics); Polarimeter; Astrophysics; Optics; Magnetic field; Mathematics; Geometry","score_opus":0.023152060127293483,"score_gpt":0.2048437403810389,"score_spread":0.1816916802537454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4212972699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95651805,0.00016472637,0.0028316549,0.00006918319,0.000032805976,0.00002533935,0.03380432,0.00028190084,0.006272028],"genre_scores_gemma":[0.91902083,0.00012857621,0.0051167333,0.00006467092,0.00002942643,0.000052851774,0.07358738,0.000097793694,0.0019016943],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984276,0.000019093615,0.0000133034955,0.000048627047,0.000056278324,0.000019938258],"domain_scores_gemma":[0.99940395,0.000077300734,0.00016237711,0.00015373438,0.00014626635,0.000056379893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030046536,0.00024572792,0.00022604824,0.0013278794,0.00026265444,0.00042345322,0.00022118914,0.0002151561,0.0014501758],"category_scores_gemma":[0.00070779276,0.00013773498,0.00014405244,0.0014862728,0.0001393638,0.00029148342,0.00045667557,0.00023736445,0.0008250401],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009165345,0.00015036677,0.866247,0.00010403808,0.00019562192,0.0002549535,0.00018782838,0.0062619406,0.051029403,0.00082398875,0.014145644,0.05968273],"study_design_scores_gemma":[0.000032733085,0.00004929152,0.9783683,0.000008494069,0.000024979607,0.00018156465,0.000058664675,0.0039551645,0.008808589,0.00017067631,0.008326759,0.0000148779445],"about_ca_topic_score_codex":0.005192949,"about_ca_topic_score_gemma":0.012471045,"teacher_disagreement_score":0.005192949,"about_ca_system_score_codex":0.00021215666,"about_ca_system_score_gemma":0.00017685085,"threshold_uncertainty_score":0.010325432},"labels":[],"label_agreement":null},{"id":"W4213035487","doi":"10.3847/1538-4357/ac45fe","title":"The Color Gradients of the Globular Cluster Systems in M87 and M49","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Shanghai Key Laboratory for Particle Physics and Cosmology; Higher Education Discipline Innovation Project; National Natural Science Foundation of China; Natural Science Foundation of Shanghai","keywords":"Virgo Cluster; Physics; Globular cluster; Astrophysics; Galaxy; Elliptical galaxy; Effective radius; Astronomy; RADIUS; Satellite galaxy; Population; Star cluster; Stars; Dwarf galaxy; Medicine","score_opus":0.004921576882501153,"score_gpt":0.19171206960082618,"score_spread":0.186790492718325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213035487","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99932015,0.00004332541,0.000031585685,0.000009227856,6.519209e-7,8.7918517e-7,0.00012060941,0.0000033180036,0.00047032879],"genre_scores_gemma":[0.9995963,0.000018576233,0.00005398622,0.000006967396,0.0000017123683,0.0000010602001,0.00024656666,0.0000018565189,0.0000730637],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989045,0.000016312051,0.000005627626,0.000028623193,0.000027721127,0.00003126681],"domain_scores_gemma":[0.99955195,0.000058835758,0.00013591841,0.000050003495,0.000092055714,0.00011109938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016151146,0.0001097283,0.00014422656,0.0012715699,0.0002443276,0.00045077535,0.00021600482,0.0001951102,0.00083102955],"category_scores_gemma":[0.0007769072,0.00008059595,0.00011791459,0.0006890252,0.00029254274,0.00025531612,0.0007697491,0.00014204599,0.00029443455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060164617,0.000012186078,0.9912397,0.000007002629,0.000029293495,0.00004937843,0.0002942763,0.00015485076,0.004543147,0.00022782848,0.00022503723,0.0031570988],"study_design_scores_gemma":[8.1680133e-7,0.0000043634604,0.99955577,0.0000010166012,0.0000026822602,0.000017868822,0.000054857377,0.0001062703,0.00012493347,0.000025359155,0.000105205945,8.4541875e-7],"about_ca_topic_score_codex":0.009169228,"about_ca_topic_score_gemma":0.011512429,"teacher_disagreement_score":0.009169228,"about_ca_system_score_codex":0.00033513538,"about_ca_system_score_gemma":0.000099810124,"threshold_uncertainty_score":0.01823169},"labels":[],"label_agreement":null},{"id":"W4213049762","doi":"10.3847/1538-4357/ac498a","title":"Estimate of the Mass and Radial Profile of the Orphan–Chenab Stream's Dwarf-galaxy Progenitor Using MilkyWay@home","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Los Alamos National Laboratory; U.S. Naval Observatory; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; New Mexico State University; University of Portsmouth; Universität Basel; University of Pittsburgh; Johns Hopkins University; Ohio State University; National Science Foundation; University of Washington; Drexel University; Alfred P. Sloan Foundation; New York Space Grant Consortium; National Aeronautics and Space Administration; Princeton University; U.S. Department of Energy; Case Western Reserve University","keywords":"Physics; Astrophysics; Galaxy; Dwarf galaxy; Milky Way; Dark matter; RADIUS; Stars; Astronomy; Dark matter halo; Virial mass; Mass ratio; Halo","score_opus":0.008176001943875646,"score_gpt":0.21567210870135345,"score_spread":0.20749610675747782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213049762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99727076,0.000023355917,0.0016579311,0.000023384599,0.0000019584522,0.000007660072,0.00018416019,0.0001348373,0.00069598167],"genre_scores_gemma":[0.9961358,0.000017557533,0.0029406454,0.00001111888,0.0000027405601,0.0000066316156,0.0005728544,0.00004613956,0.00026645794],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993145,0.000010511634,0.0000028038496,0.000020922731,0.000018138137,0.00001613024],"domain_scores_gemma":[0.99970835,0.00004282577,0.00006425379,0.00003840071,0.00006128216,0.00008492508],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034894058,0.0002907518,0.00034448763,0.0005856711,0.00051298644,0.00038943085,0.00068330375,0.0003103441,0.0011697509],"category_scores_gemma":[0.0010087731,0.00025253513,0.00043789862,0.0004384174,0.00019621072,0.00026372517,0.00053781667,0.0002477213,0.000512411],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001825863,0.00006923073,0.84385246,0.000032274223,0.00012405375,0.00056617777,0.00020623172,0.13160308,0.010190842,0.0012794313,0.0009433274,0.010950394],"study_design_scores_gemma":[0.000090788526,0.00010502547,0.25946623,0.000018979561,0.00006294882,0.00028538785,0.0002506092,0.72858596,0.007748795,0.0007617116,0.0025899392,0.000033656757],"about_ca_topic_score_codex":0.022215685,"about_ca_topic_score_gemma":0.022352556,"teacher_disagreement_score":0.022215685,"about_ca_system_score_codex":0.00081129867,"about_ca_system_score_gemma":0.0005919749,"threshold_uncertainty_score":0.044172764},"labels":[],"label_agreement":null},{"id":"W4213135393","doi":"10.3847/1538-4357/ac441c","title":"A Wide and Deep Exploration of Radio Galaxies with Subaru HSC (WERGS). VI. Distant Filamentary Structures Pointed Out by High-z Radio Galaxies at z ∼ 4","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; National Central University; Eötvös Loránd Tudományegyetem; Academia Sinica; Space Telescope Science Institute; Queen's University; Ministry of Education, Culture, Sports, Science and Technology; Los Alamos National Laboratory; Princeton University; Johns Hopkins University; Japan Society for the Promotion of Science; Queen's University Belfast; National Aeronautics and Space Administration; Smithsonian Institution; Japan Science and Technology Agency; Cabinet Office, Government of Japan; Durham University; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Halo; Luminosity; Radio galaxy; Stars","score_opus":0.005740753206066377,"score_gpt":0.19017719968756794,"score_spread":0.18443644648150156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213135393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983535,0.00013640303,0.00034650764,0.000018881177,0.0000015959284,0.000004452264,0.00034516727,0.000025501053,0.0007680746],"genre_scores_gemma":[0.99849546,0.00004551208,0.00055466907,0.0000114761315,0.000005209431,0.000004236074,0.00063073594,0.000006958966,0.00024564937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998753,0.000019705012,0.0000066943135,0.000031263502,0.000021898479,0.000045084584],"domain_scores_gemma":[0.99953926,0.000045472494,0.0001823626,0.0000571092,0.000038583246,0.00013724489],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024055617,0.00024302585,0.00019807558,0.0017775012,0.0003382823,0.00046893113,0.0002288409,0.0001452145,0.0011868841],"category_scores_gemma":[0.00032139762,0.000115204835,0.00025264904,0.0010032539,0.00021560666,0.00030268237,0.000679956,0.00016714484,0.00026685518],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004582608,0.000018975054,0.9821293,0.000012558357,0.000048538444,0.00010932873,0.00019614305,0.00025314436,0.0063984194,0.00016261994,0.00020840489,0.010416832],"study_design_scores_gemma":[6.861338e-7,0.0000103082775,0.99905616,0.0000018149856,0.000008707238,0.00003088901,0.000087889675,0.00016164214,0.00025689328,0.000042943582,0.00034091208,0.0000012003234],"about_ca_topic_score_codex":0.0028859451,"about_ca_topic_score_gemma":0.0060483413,"teacher_disagreement_score":0.0028859451,"about_ca_system_score_codex":0.00015677308,"about_ca_system_score_gemma":0.000107857166,"threshold_uncertainty_score":0.0057382584},"labels":[],"label_agreement":null},{"id":"W4213145174","doi":"10.3847/1538-4357/ac4419","title":"The LEGA-C of Nature and Nurture in Stellar Populations at z ∼ 0.6–1.0: D<sub> n </sub>4000 and Hδ Reveal Different Assembly Histories for Quiescent Galaxies in Different Environments","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"East Asian Core Observatories Association; European Commission","keywords":"Physics; Galaxy; Astrophysics; Stellar mass; Satellite galaxy; Star formation; Galaxy formation and evolution; Astronomy","score_opus":0.006467661078817227,"score_gpt":0.2040031915139518,"score_spread":0.19753553043513458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213145174","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980336,0.00006779417,0.00014311938,0.000039504714,0.000001304171,0.0000012214069,0.00060412905,0.000013959704,0.0010953802],"genre_scores_gemma":[0.9991041,0.000016139227,0.00009145247,0.000023542754,0.0000019979173,0.0000015157777,0.0005605101,0.0000066386515,0.00019396488],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998914,0.00001160606,0.000004692681,0.000046368274,0.000016458234,0.000029463856],"domain_scores_gemma":[0.9991823,0.0001831929,0.0002738144,0.00007139559,0.00007224344,0.00021699393],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022217982,0.00012994555,0.00017597899,0.00087979983,0.00023751636,0.000825206,0.00019677595,0.00026038248,0.0022655225],"category_scores_gemma":[0.0006485086,0.00012582932,0.00023257903,0.0006146122,0.00037938802,0.0003213924,0.0008430588,0.00019799305,0.00032455652],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000118921,0.000011778154,0.97817844,0.000015437006,0.00007373726,0.00005491501,0.00030806893,0.0002985878,0.014766692,0.00050842646,0.00027750662,0.005387415],"study_design_scores_gemma":[0.0000010152227,0.0000036407805,0.99922514,0.0000018202122,0.0000034272266,0.000023578976,0.00006190156,0.00023558828,0.00017939367,0.000051621002,0.00021130285,0.0000015691496],"about_ca_topic_score_codex":0.0055897,"about_ca_topic_score_gemma":0.0091091255,"teacher_disagreement_score":0.0055897,"about_ca_system_score_codex":0.00022294569,"about_ca_system_score_gemma":0.00011560088,"threshold_uncertainty_score":0.011114299},"labels":[],"label_agreement":null},{"id":"W4213425166","doi":"10.3847/1538-4357/ac4ae4","title":"4FGL J1120.0–2204: A Unique Gamma-Ray-bright Neutron Star Binary with an Extremely Low-mass Proto-white Dwarf","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Millisecond pulsar; White dwarf; Astrophysics; Neutron star; Pulsar; Fermi Gamma-ray Space Telescope; Astronomy; Millisecond; Binary number; Stars","score_opus":0.011608281261108622,"score_gpt":0.2194384247091499,"score_spread":0.20783014344804127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4213425166","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983783,0.00007911511,0.0002033479,0.00007340917,0.000013787691,0.000003687841,0.00008557964,0.000027406792,0.0011353177],"genre_scores_gemma":[0.99870074,0.000016532747,0.00029854014,0.000041600044,0.000012113983,0.0000020981456,0.00023445695,0.0000056619256,0.00068828004],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992776,0.0000059037175,0.0000044236963,0.000022232767,0.000013781461,0.000025853084],"domain_scores_gemma":[0.9998425,0.000009829608,0.000050616756,0.000015472595,0.000012511797,0.000069026864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011094446,0.00026279545,0.0003161833,0.0007024599,0.0009543433,0.00058181654,0.00033737873,0.00067554374,0.0018232993],"category_scores_gemma":[0.00024854887,0.00015095268,0.00015693132,0.0003262407,0.00038687617,0.0002729443,0.00063579687,0.00036651827,0.0005807182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010580249,0.00058319484,0.67450386,0.00010725372,0.00009921438,0.04042661,0.00092218,0.0008300403,0.24861729,0.0024380148,0.002466363,0.027948048],"study_design_scores_gemma":[0.00008768466,0.00074099854,0.87652415,0.000025657322,0.00006544058,0.081232846,0.0007923478,0.003134605,0.015438833,0.0016637889,0.020236047,0.000057560206],"about_ca_topic_score_codex":0.0019734446,"about_ca_topic_score_gemma":0.0025681013,"teacher_disagreement_score":0.0019734446,"about_ca_system_score_codex":0.00048055506,"about_ca_system_score_gemma":0.000165872,"threshold_uncertainty_score":0.0060995817},"labels":[],"label_agreement":null},{"id":"W4214569019","doi":"10.3847/1538-4357/ac4d98","title":"Can a Single Population Account for the Discriminant Properties in Fast Radio Bursts?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Key Research and Development Program of China; China Postdoctoral Science Foundation; National Natural Science Foundation of China","keywords":"Physics; Maser; Astrophysics; Synchrotron radiation; Spectral index; Population; Discriminant; Radiation; Luminosity; Optics; Astronomy; Spectral line; Galaxy; Artificial intelligence","score_opus":0.0221963891836003,"score_gpt":0.22741281865102767,"score_spread":0.20521642946742735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214569019","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9780662,0.0004204089,0.016936291,0.00069477106,0.000072569,0.00006303954,0.0003389341,0.0001488545,0.0032589084],"genre_scores_gemma":[0.99797565,0.000048661008,0.0013365325,0.00008524406,0.000040808514,0.000014928664,0.00017834017,0.000022122384,0.00029772482],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9988722,0.00024020886,0.00006134413,0.00042931808,0.00018334629,0.00021352722],"domain_scores_gemma":[0.9919932,0.0031483471,0.0016460767,0.0013659111,0.00094698125,0.00089942274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0040852167,0.000541984,0.001080291,0.002221384,0.0009202715,0.0025165777,0.0013232575,0.001032653,0.0042979917],"category_scores_gemma":[0.011852479,0.00030043183,0.0009993636,0.0010874496,0.0015855462,0.00211425,0.0016734615,0.0010676221,0.0007421075],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000582514,0.00013569463,0.9480361,0.00006386379,0.00037799648,0.0002103502,0.0005946529,0.0032427295,0.0057654018,0.0080730235,0.001058017,0.031859633],"study_design_scores_gemma":[0.00006283486,0.00019065614,0.89730996,0.00002881523,0.00022538989,0.00047405888,0.00093189266,0.06628649,0.00095394824,0.031791423,0.0016763131,0.00006823119],"about_ca_topic_score_codex":0.005259747,"about_ca_topic_score_gemma":0.0033103263,"teacher_disagreement_score":0.005259747,"about_ca_system_score_codex":0.00062427274,"about_ca_system_score_gemma":0.00072497124,"threshold_uncertainty_score":0.021604955},"labels":[],"label_agreement":null},{"id":"W4214739086","doi":"10.3847/1538-4357/ac4ccc","title":"The ALMaQUEST Survey. VII. Star Formation Scaling Relations of Green Valley Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; Ministry of Science and Technology, Taiwan","keywords":"Algorithm; Physics; Computer science","score_opus":0.01160888978007863,"score_gpt":0.217180372454402,"score_spread":0.20557148267432337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214739086","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9648528,0.0005095078,0.00025960893,0.00035799886,0.0000134840575,0.0000141205965,0.02703029,0.00012965928,0.006832597],"genre_scores_gemma":[0.97860867,0.0001384066,0.0005869126,0.00014177612,0.000027853603,0.000021550339,0.01825871,0.000057972396,0.0021582446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998178,0.000033614742,0.0000072290322,0.00006496476,0.000038912574,0.00003752002],"domain_scores_gemma":[0.99889,0.00015258291,0.0003957681,0.00013238617,0.00017367135,0.00025559898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044176306,0.00014395427,0.00013747846,0.0016939153,0.0002185144,0.00064960786,0.0003617152,0.00018521497,0.0030767675],"category_scores_gemma":[0.0010681037,0.000084218205,0.00021380109,0.0017776983,0.00016453589,0.00041228568,0.000468479,0.00023898379,0.0009154877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000099417404,0.000035477624,0.9683689,0.000029997744,0.000039613267,0.00008414793,0.00034347372,0.00034818312,0.0010308094,0.00072891644,0.010793408,0.01809775],"study_design_scores_gemma":[0.000011500167,0.000016585765,0.9934754,0.0000057482443,0.000005862144,0.000044984674,0.0001200097,0.00053084374,0.0001480069,0.00022808943,0.0054082633,0.000004758105],"about_ca_topic_score_codex":0.037359893,"about_ca_topic_score_gemma":0.066575706,"teacher_disagreement_score":0.037359893,"about_ca_system_score_codex":0.0005016811,"about_ca_system_score_gemma":0.00025657285,"threshold_uncertainty_score":0.07428485},"labels":[],"label_agreement":null},{"id":"W4214744376","doi":"10.3847/1538-4357/ac4bbe","title":"B-fields in Star-forming Region Observations (BISTRO): Magnetic Fields in the Filamentary Structures of Serpens Main","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; University of Manitoba; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics; McMaster University; Queen's University","funders":"Science and Engineering Research Board; Japan Society for the Promotion of Science; National Research Foundation; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; Ministry of Education, Science and Technology; Seoul National University; Department of Science and Technology, Ministry of Science and Technology, India; National Natural Science Foundation of China; National Research Foundation of Korea","keywords":"Serpens; Physics; Astrophysics; Magnetic field; Molecular cloud; Star formation; James Clerk Maxwell Telescope; Young stellar object; Stars","score_opus":0.020456018503082898,"score_gpt":0.23771457943172564,"score_spread":0.21725856092864274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214744376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.989781,0.00013956975,0.00082851085,0.000054156433,0.000016822478,0.000011826501,0.002839653,0.00046276997,0.005865723],"genre_scores_gemma":[0.9953107,0.000083230334,0.0013141182,0.000025857427,0.000027651931,0.000005038697,0.0025271669,0.000046830413,0.0006592849],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994814,0.00000768581,0.0000035977548,0.000016263317,0.00001223369,0.000012017097],"domain_scores_gemma":[0.99984777,0.000024533649,0.000050848677,0.000023545004,0.000016371732,0.00003685284],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011211056,0.00014335607,0.00008688571,0.00094522367,0.00009684306,0.00024737106,0.00013458406,0.00010830342,0.0022610356],"category_scores_gemma":[0.0003421052,0.00007628144,0.00009774224,0.00045893522,0.00009080222,0.00014022262,0.00019482762,0.00011409159,0.0004490947],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083240797,0.00011695008,0.7590374,0.00017801068,0.00011903232,0.0009454487,0.0004919042,0.0046849707,0.14081356,0.00065462093,0.007983644,0.08414209],"study_design_scores_gemma":[0.000025764823,0.00004409185,0.98272103,0.000015573953,0.000025763053,0.00015876783,0.000069092486,0.002121805,0.009799881,0.00010371289,0.00490894,0.000005583992],"about_ca_topic_score_codex":0.0038697694,"about_ca_topic_score_gemma":0.0062293843,"teacher_disagreement_score":0.0038697694,"about_ca_system_score_codex":0.00017775175,"about_ca_system_score_gemma":0.00007940981,"threshold_uncertainty_score":0.007694483},"labels":[],"label_agreement":null},{"id":"W4214812735","doi":"10.3847/1538-4357/ac496a","title":"Toward a More Complete Optical Census of Active Galactic Nuclei via Spatially Resolved Spectroscopy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; University of Oxford; York University; Carnegie Institution for Science; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Max-Planck-Institut für Astrophysik","keywords":"Active galactic nucleus; Physics; Astrophysics; Galaxy; Spectral line; Astronomy; Spectroscopy; Extragalactic astronomy; Observatory; Luminous infrared galaxy; Luminosity; Line (geometry); Emission spectrum; Flux (metallurgy); Chemistry","score_opus":0.01428674608371711,"score_gpt":0.23256964486529644,"score_spread":0.21828289878157933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214812735","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95389044,0.0005804148,0.039313506,0.00014801728,0.000012236291,0.000035370496,0.0025570372,0.0003940718,0.003068866],"genre_scores_gemma":[0.9608883,0.000271284,0.035296198,0.00010174916,0.000038208153,0.000025882804,0.0028738,0.0000561879,0.00044836348],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99966073,0.00007095289,0.000015778509,0.00011548015,0.00008076505,0.000056311674],"domain_scores_gemma":[0.9982687,0.0003087916,0.00049297255,0.00037332627,0.0003850129,0.00017115724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006969921,0.00035499077,0.00035983865,0.0036879405,0.00030293732,0.0012387383,0.0004967677,0.00032699615,0.0012756493],"category_scores_gemma":[0.0016408416,0.000283638,0.00051408855,0.00148815,0.0002954378,0.0011045745,0.001086471,0.00031306676,0.00057074614],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018369088,0.00019826065,0.7151946,0.00015725076,0.00028670405,0.00032364886,0.000479905,0.015203665,0.19170171,0.004746608,0.0018486808,0.06967536],"study_design_scores_gemma":[0.00002760074,0.00016286744,0.8630232,0.000057219906,0.00012121855,0.0007384112,0.00083647383,0.08619483,0.03191365,0.0058597345,0.010998482,0.00006624086],"about_ca_topic_score_codex":0.0053764274,"about_ca_topic_score_gemma":0.007892377,"teacher_disagreement_score":0.0053764274,"about_ca_system_score_codex":0.00038347198,"about_ca_system_score_gemma":0.0002654367,"threshold_uncertainty_score":0.010690272},"labels":[],"label_agreement":null},{"id":"W4214818963","doi":"10.3847/1538-4357/ac4ae7","title":"CHANG-ES. XXIV. First Detection of a Radio Nuclear Ring and Potential LLAGN in NGC 5792","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"National Key Research and Development Program of China; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Star formation; Astronomy; Ring (chemistry)","score_opus":0.00456374340920274,"score_gpt":0.17667826922348445,"score_spread":0.17211452581428172,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214818963","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99075705,0.00029483234,0.0005764216,0.00006236135,0.000015751713,0.000008102095,0.0005651413,0.00006735267,0.0076531544],"genre_scores_gemma":[0.99413294,0.000069869435,0.0005134077,0.00003350355,0.000010592821,0.0000067480955,0.0011453736,0.000010465029,0.0040770457],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995005,0.0000036848508,0.0000024399783,0.000016103902,0.000011408284,0.000016303538],"domain_scores_gemma":[0.9998568,0.000011956353,0.000030301097,0.000024636403,0.000025740104,0.000050596293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011721058,0.00013970387,0.00010042314,0.00036276295,0.00030077746,0.00048317408,0.00012755979,0.00017871449,0.0064332965],"category_scores_gemma":[0.00015647245,0.00009570569,0.00009896022,0.00022822383,0.00016131737,0.00011846333,0.00038951734,0.00014897891,0.0013909355],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045313136,0.0000662258,0.66130584,0.0000827286,0.00006129146,0.003936063,0.00045451592,0.00031424302,0.27738684,0.0007329924,0.002180391,0.05302569],"study_design_scores_gemma":[0.000012473534,0.00006825336,0.96861994,0.000015547284,0.000023646851,0.0014126073,0.00016539026,0.0003761898,0.0144925825,0.00012505689,0.014682706,0.0000056451345],"about_ca_topic_score_codex":0.002609481,"about_ca_topic_score_gemma":0.0037248253,"teacher_disagreement_score":0.0064332965,"about_ca_system_score_codex":0.00023370472,"about_ca_system_score_gemma":0.00007827574,"threshold_uncertainty_score":0.021521568},"labels":[],"label_agreement":null},{"id":"W4214927640","doi":"10.3847/1538-4357/ac4709","title":"Less Than 1% of Core-collapse Supernovae in the Local Universe Occur in Elliptical Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Science and Technology Facilities Council; Queen's University; European Commission; Horizon 2020 Framework Programme; Queen's University Belfast; Nuclear Safety and Security Commission; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration; Royal Astronomical Society; Wenner-Gren Stiftelserna; Space Telescope Science Institute; Vetenskapsrådet; National Science Foundation","keywords":"Supernova; Astrophysics; Physics; Photometry (optics); Galaxy; Ejecta; Light curve; Stars; Astronomy","score_opus":0.017962786619253414,"score_gpt":0.2328693909236976,"score_spread":0.2149066043044442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214927640","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99732226,0.00022015483,0.000120202756,0.000012718571,0.0000030357296,0.0000046949344,0.000697393,0.000037922655,0.0015815762],"genre_scores_gemma":[0.9982961,0.000121823316,0.0000732873,0.0000103296625,0.000006732873,0.000002335315,0.0008499137,0.000005621182,0.00063378166],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987316,0.000012174361,0.000009876997,0.00003593167,0.00003175401,0.00003708803],"domain_scores_gemma":[0.99964106,0.000032494343,0.00011940379,0.00006841401,0.000045634402,0.000092933355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016320634,0.00015539596,0.00015269568,0.0008980592,0.00018926282,0.0003317287,0.00018949849,0.00012232906,0.003832846],"category_scores_gemma":[0.00051897357,0.000086942404,0.0001502781,0.0004803084,0.00015683887,0.00023471026,0.00032959986,0.000070785056,0.00089602324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000051308543,0.000019353884,0.9908392,0.0000107736505,0.00002468153,0.00009280628,0.00006568812,0.00003782129,0.002418697,0.000047361318,0.0003573975,0.006034927],"study_design_scores_gemma":[0.0000019826525,0.000024054876,0.9978167,0.000003900779,0.000008502131,0.00025666782,0.0000863194,0.000059084738,0.00055344927,0.000023071174,0.0011652776,0.000001029087],"about_ca_topic_score_codex":0.0044678347,"about_ca_topic_score_gemma":0.010905547,"teacher_disagreement_score":0.0044678347,"about_ca_system_score_codex":0.00018024941,"about_ca_system_score_gemma":0.00008380514,"threshold_uncertainty_score":0.012822151},"labels":[],"label_agreement":null},{"id":"W4214937809","doi":"10.3847/1538-4357/ac474f","title":"The Gas–Star Formation Cycle in Nearby Star-forming Galaxies. II. Resolved Distributions of CO and Hα Emission for 49 PHANGS Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Institut National de Physique Nucléaire et de Physique des Particules; National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; Agencia Nacional de Investigación y Desarrollo; Ministerio de Ciencia e Innovación; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; National Astronomical Observatory of Japan; European Commission; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; Ministerio de Ciencia, Innovación y Universidades; Agencia Estatal de Investigación; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Astronomy","score_opus":0.008378235115030871,"score_gpt":0.2272317420467225,"score_spread":0.21885350693169164,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4214937809","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996277,0.000025043224,0.000027244114,0.0000029529592,2.6190062e-7,0.0000017463615,0.0001713654,0.0000035051946,0.00014011817],"genre_scores_gemma":[0.9993993,0.000017574836,0.00007461855,0.0000019610754,0.0000014410999,0.0000019373006,0.00041410452,0.0000014879901,0.00008757527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999094,0.000015388923,0.0000063159873,0.000027950058,0.000014865328,0.000026026715],"domain_scores_gemma":[0.9995751,0.0000690718,0.00014165587,0.000040847655,0.000051616338,0.00012177808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001870745,0.00013993838,0.00015795458,0.0010317247,0.0002519351,0.00041575666,0.00019762998,0.0002181836,0.0009301831],"category_scores_gemma":[0.00042967597,0.00012946245,0.00019937826,0.0006553571,0.0002653302,0.00025935005,0.00033568038,0.00010566145,0.00026946914],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000085791056,0.00002486817,0.99047196,0.000006767064,0.000021079311,0.000061084604,0.0002436617,0.00020688986,0.006485806,0.00005101561,0.000045127294,0.0022959677],"study_design_scores_gemma":[0.0000011708266,0.0000143275975,0.99943775,5.4510116e-7,0.0000023794626,0.000022013077,0.000052323627,0.00020106783,0.00019807782,0.000007840138,0.00006176964,8.2427766e-7],"about_ca_topic_score_codex":0.010227444,"about_ca_topic_score_gemma":0.013110902,"teacher_disagreement_score":0.010227444,"about_ca_system_score_codex":0.00033286758,"about_ca_system_score_gemma":0.00009776937,"threshold_uncertainty_score":0.020335793},"labels":[],"label_agreement":null},{"id":"W4220655658","doi":"10.3847/1538-4357/ac4886","title":"Bicep/Keck XV: The Bicep3 Cosmic Microwave Background Polarimeter and the First Three-year Data Set","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"SLAC National Accelerator Laboratory; Jet Propulsion Laboratory; Canada Foundation for Innovation; Harvard University; U.S. Department of Energy; Gordon and Betty Moore Foundation; W. M. Keck Foundation; California Institute of Technology; National Aeronautics and Space Administration; Advanced Research Projects Agency; National Science Foundation","keywords":"Physics; Polarimeter; Cosmic microwave background; Astronomy; Astrophysics; COSMIC cancer database; Cosmic background radiation; Cosmic infrared background; Polarimetry; Optics","score_opus":0.022217792216729912,"score_gpt":0.256207948044871,"score_spread":0.2339901558281411,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220655658","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.38992453,0.0017398791,0.019938825,0.0015986149,0.0007196865,0.00073899137,0.539288,0.009486593,0.036564887],"genre_scores_gemma":[0.27191114,0.00051856134,0.04027438,0.0007732509,0.0002020956,0.0010146115,0.6771623,0.0019333845,0.0062103663],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9987777,0.000103313396,0.000046007666,0.00019067884,0.00067252223,0.00020993304],"domain_scores_gemma":[0.9976955,0.00014977551,0.00019265994,0.00061110535,0.0010165861,0.00033441416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002406178,0.0008965318,0.00078648125,0.001665824,0.001230343,0.0018610202,0.0010452968,0.0008659946,0.0036817817],"category_scores_gemma":[0.0023406078,0.00054882886,0.0006657436,0.0021388258,0.00047202356,0.0011856807,0.0024260532,0.0018188562,0.002945381],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0034515448,0.0007734822,0.20119345,0.00071567,0.0011153396,0.0015939589,0.000688517,0.030180747,0.046026077,0.007011681,0.57683784,0.1304117],"study_design_scores_gemma":[0.00063078915,0.00036302092,0.42317268,0.00030039094,0.00026579146,0.0005147782,0.00022006096,0.0179931,0.05539804,0.003095062,0.4977509,0.0002953375],"about_ca_topic_score_codex":0.029305035,"about_ca_topic_score_gemma":0.02696569,"teacher_disagreement_score":0.029305035,"about_ca_system_score_codex":0.0011989458,"about_ca_system_score_gemma":0.0022088417,"threshold_uncertainty_score":0.058268905},"labels":[],"label_agreement":null},{"id":"W4220688262","doi":"10.3847/1538-4357/ac496f","title":"The Evolution of the Orbital Lightcurve of Hercules X-1 with 35 Day Phase","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Neutron star; Physics; Astrophysics; Orbital period; Eclipse; Phase (matter); Light curve; Orbital inclination; Photoelectric effect; Orbital elements; Astronomy; Binary number; Optics","score_opus":0.007769790211586034,"score_gpt":0.22159862662205335,"score_spread":0.21382883641046732,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220688262","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99756086,0.000108754975,0.00014147913,0.000022192307,0.00000437833,0.00000411079,0.0007067382,0.000056843353,0.0013945191],"genre_scores_gemma":[0.9974383,0.00003993378,0.00011815481,0.000007659802,0.0000074048658,0.0000041966446,0.0018147946,0.000019210242,0.0005504123],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999254,0.000007746592,0.000002883707,0.000023642373,0.000017634164,0.000022746624],"domain_scores_gemma":[0.99960893,0.000054956854,0.00011192994,0.0000379825,0.000108243774,0.00007807594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017290922,0.00024421114,0.00016042814,0.0013781906,0.00022911732,0.00046288062,0.00014175603,0.00021501277,0.0014279222],"category_scores_gemma":[0.00043985134,0.00008553944,0.00015629873,0.00076178665,0.00013325956,0.00016673241,0.00034904122,0.00020601644,0.0002802973],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010087414,0.0001509039,0.8581928,0.000094505136,0.00012798987,0.0005211621,0.00073131657,0.0042865295,0.08948393,0.00078853447,0.00350108,0.041112546],"study_design_scores_gemma":[0.0000029582582,0.00003731301,0.99653316,0.000004005398,0.0000063433527,0.00006182906,0.00005006803,0.0011464419,0.0010933026,0.000038068974,0.0010217282,0.0000048197476],"about_ca_topic_score_codex":0.004161649,"about_ca_topic_score_gemma":0.0043144133,"teacher_disagreement_score":0.004161649,"about_ca_system_score_codex":0.0003157417,"about_ca_system_score_gemma":0.00009433515,"threshold_uncertainty_score":0.008274853},"labels":[],"label_agreement":null},{"id":"W4220708542","doi":"10.3847/1538-4357/ac54ad","title":"Stellar Abundance Maps of the Milky Way Disk","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Flatiron Health; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Max-Planck-Institut für Astrophysik","keywords":"Milky Way; Astrophysics; Stars; Physics; Abundance (ecology); Red clump; Red-giant branch; Astronomy; Giant star; Metallicity; Ecology; Biology","score_opus":0.008930033850637991,"score_gpt":0.20822655236542187,"score_spread":0.1992965185147839,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220708542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996935,0.00008584867,0.0006076851,0.0000148231165,9.0555005e-7,0.0000036522706,0.0010029053,0.00011351201,0.0012356427],"genre_scores_gemma":[0.99579066,0.000050837934,0.0017391132,0.0000049230343,0.0000027407189,0.0000046774935,0.0019876894,0.000019316727,0.0004000403],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990606,0.00001103306,0.000005217835,0.000033917648,0.000028489461,0.0000152435805],"domain_scores_gemma":[0.99961346,0.00007245861,0.000085742664,0.000051656134,0.00012945534,0.00004720704],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014638675,0.00012803198,0.00016288481,0.0020744898,0.00015462382,0.00042492125,0.00019906407,0.00016419376,0.0017146923],"category_scores_gemma":[0.00065683655,0.000098649485,0.0002540515,0.0013284228,0.00012146948,0.00017451953,0.00053822616,0.000089346955,0.00039875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024294635,0.00004889606,0.8987671,0.00010692479,0.00014912151,0.00022685724,0.0008943004,0.016746016,0.029514229,0.0009311406,0.0013648364,0.051007558],"study_design_scores_gemma":[0.0000133536405,0.000031420062,0.97396356,0.000010043413,0.000019907724,0.0001080362,0.00027149264,0.018743556,0.0033758418,0.00033471835,0.003119542,0.000008633771],"about_ca_topic_score_codex":0.01223498,"about_ca_topic_score_gemma":0.013016919,"teacher_disagreement_score":0.01223498,"about_ca_system_score_codex":0.00031469527,"about_ca_system_score_gemma":0.00014130688,"threshold_uncertainty_score":0.024327517},"labels":[],"label_agreement":null},{"id":"W4220710530","doi":"10.3847/1538-4357/ac503d","title":"The Farthest Quasar Mini-Broad Absorption Line Outflow from Its Central Source: Very Large Telescope/UVES Observation of SDSS J0242+0049","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Virginia Space Grant Consortium; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Quasar; Astrophysics; Outflow; Telescope; Active galactic nucleus; Astronomy; Line (geometry); Luminosity; Ionization; Absorption (acoustics); Galaxy; Optics","score_opus":0.01123197759263957,"score_gpt":0.2119869141458796,"score_spread":0.20075493655324003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220710530","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988618,0.00008516675,0.00012127989,0.000018963154,0.0000033341776,0.0000025284467,0.00029975554,0.000025310148,0.0005819228],"genre_scores_gemma":[0.99897134,0.000024959587,0.00013768538,0.000016564469,0.000009141882,0.0000018831045,0.0007235115,0.00000391407,0.00011101822],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987495,0.000011762761,0.0000070042865,0.000036960875,0.00003419408,0.00003501879],"domain_scores_gemma":[0.99938786,0.00005102611,0.00023344763,0.000046307185,0.00006171651,0.00021953811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026874073,0.0001943669,0.00028856847,0.0013367974,0.00045302243,0.0007259256,0.00025791663,0.00027945326,0.0008997781],"category_scores_gemma":[0.0004280905,0.0001456691,0.0002988663,0.00072203984,0.00027204357,0.00029817357,0.0005531339,0.00023711835,0.00018970565],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014603026,0.00015124088,0.9580719,0.00003551027,0.00014784337,0.0004657414,0.0003102986,0.0013181083,0.03141851,0.00027796743,0.0010815415,0.0065752803],"study_design_scores_gemma":[0.0000068666177,0.000017599745,0.9978898,0.0000035700746,0.000015048691,0.000085984415,0.00006690984,0.0010823181,0.00042899075,0.000028635584,0.0003693599,0.000004978635],"about_ca_topic_score_codex":0.010296772,"about_ca_topic_score_gemma":0.019021586,"teacher_disagreement_score":0.010296772,"about_ca_system_score_codex":0.00033228926,"about_ca_system_score_gemma":0.00024020595,"threshold_uncertainty_score":0.020473659},"labels":[],"label_agreement":null},{"id":"W4220713584","doi":"10.3847/1538-4357/ac4cae","title":"Misaligned Rotations of the Envelope, Outflow, and Disks in the Multiple Protostellar System of VLA 1623–2417: FAUST. III","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; National Institutes of Natural Sciences; Japan Society for the Promotion of Science; National Science Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; European Commission; Associated Universities; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Circumbinary planet; Astrophysics; Rotation (mathematics); Outflow; Velocity gradient; Envelope (radar); Protostar; Astronomy; Stars; Star formation; Geometry; Mechanics","score_opus":0.010037737693057764,"score_gpt":0.225384846963494,"score_spread":0.21534710927043624,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220713584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995962,0.00004145101,0.00015461566,0.00000584401,0.0000010838958,0.0000014105424,0.000060407747,0.000018129134,0.000121002005],"genre_scores_gemma":[0.999551,0.0000057737375,0.00024756682,0.0000057432853,0.0000013889768,0.0000013757488,0.00011695275,0.0000058302253,0.000064303866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998903,0.0000146657685,0.000003398386,0.00003852105,0.000019751555,0.00003319145],"domain_scores_gemma":[0.99973625,0.00002383334,0.00009792546,0.000033207074,0.000024176914,0.000084584084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017440009,0.00025644028,0.00023321944,0.0004984261,0.0004594401,0.00038466757,0.0002899114,0.0002463942,0.0004829966],"category_scores_gemma":[0.00025444952,0.00015356446,0.00016591091,0.0003709971,0.00030146475,0.00019366248,0.00031436034,0.00026081703,0.00017155305],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000643485,0.00017592454,0.6510973,0.000036438905,0.00013971311,0.00090708805,0.00041081398,0.0027426674,0.33200485,0.00022463505,0.00039134515,0.0112257665],"study_design_scores_gemma":[0.000011397851,0.000086160595,0.98819155,0.0000025043705,0.000015094172,0.00031800944,0.00010284094,0.0035578401,0.007146232,0.00005136888,0.00050781644,0.00000911849],"about_ca_topic_score_codex":0.007683247,"about_ca_topic_score_gemma":0.0074079,"teacher_disagreement_score":0.007683247,"about_ca_system_score_codex":0.00045340584,"about_ca_system_score_gemma":0.00015358905,"threshold_uncertainty_score":0.015277028},"labels":[],"label_agreement":null},{"id":"W4220736168","doi":"10.3847/1538-4357/ac558e","title":"The Dawn of Disk Formation in a Milky Way-sized Galaxy Halo: Thin Stellar Disks at z &gt; 4","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Goddard Space Flight Center; National Science Foundation; Centro Svizzero di Calcolo Scientifico; National Supercomputing Centre Singapore; National Aeronautics and Space Administration; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung","keywords":"Physics; Astrophysics; Thick disk; Thin disk; Galaxy; Milky Way; Redshift; Astronomy; Galaxy formation and evolution; Star formation; Halo; Interacting galaxy","score_opus":0.007703066924396678,"score_gpt":0.20857984368618235,"score_spread":0.20087677676178567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220736168","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982659,0.000046686506,0.00026704583,0.00013586877,0.000007452777,0.0000049081045,0.0001493048,0.000054465574,0.0010683422],"genre_scores_gemma":[0.998818,0.000029790779,0.00046364035,0.000043818978,0.000005581785,0.0000042964575,0.0002146915,0.000019859383,0.00040027345],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999013,0.000027104013,0.0000025907498,0.000013746287,0.00001511306,0.000040033614],"domain_scores_gemma":[0.9995511,0.00012880322,0.000048478974,0.000035123627,0.000044298664,0.0001920651],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043678595,0.0003429495,0.00044384398,0.00034905953,0.00058489514,0.0007700866,0.0007819035,0.00075966626,0.0017916424],"category_scores_gemma":[0.0016070534,0.00030177707,0.00056472776,0.00025815135,0.0009880249,0.00049586553,0.0009951356,0.0008231033,0.00016023261],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072819984,0.00032509252,0.13152644,0.000078984864,0.00027069415,0.0012113386,0.000586931,0.8437891,0.009128738,0.007483142,0.0019452227,0.002926091],"study_design_scores_gemma":[0.0003782949,0.0003130659,0.058181837,0.000019321626,0.000087763445,0.00011868325,0.00035653074,0.934895,0.0022274484,0.0020847437,0.0012978015,0.000039530627],"about_ca_topic_score_codex":0.037090104,"about_ca_topic_score_gemma":0.023196213,"teacher_disagreement_score":0.037090104,"about_ca_system_score_codex":0.0013066131,"about_ca_system_score_gemma":0.00073390186,"threshold_uncertainty_score":0.07374841},"labels":[],"label_agreement":null},{"id":"W4220776121","doi":"10.3847/1538-4357/ac4e18","title":"LEGA-C: Analysis of Dynamical Masses from Ionized Gas and Stellar Kinematics at z ∼ 0.8","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Velocity dispersion; Stellar kinematics; Star formation; Redshift; Kinematics; RADIUS; Galaxy formation and evolution; Classical mechanics","score_opus":0.006315833355926147,"score_gpt":0.20703211784235173,"score_spread":0.2007162844864256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220776121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98453647,0.00013316786,0.0011635885,0.00004703282,0.000005773696,0.000012844747,0.011547227,0.00038885078,0.002165003],"genre_scores_gemma":[0.97839326,0.00002206777,0.0021495805,0.000037507336,0.000009974289,0.000020327088,0.018928835,0.00009817288,0.00034025888],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996865,0.00007012345,0.000014355566,0.000102423866,0.000057354184,0.00006939479],"domain_scores_gemma":[0.9985306,0.0004162262,0.00035845165,0.0002329124,0.00016510562,0.00029667275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007254284,0.00036685335,0.00030531108,0.00225313,0.00026739945,0.00086403993,0.00059445476,0.0003772493,0.0013419361],"category_scores_gemma":[0.0016443689,0.00014607803,0.0005893138,0.0011649755,0.00019722282,0.00027146892,0.0008019002,0.00021890104,0.00085498736],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059972686,0.00009127752,0.9398569,0.000095902455,0.0004614478,0.00024300965,0.00028706863,0.01023243,0.019486105,0.0007408464,0.0041577364,0.023747465],"study_design_scores_gemma":[0.00002152343,0.000039544742,0.97618973,0.000011335531,0.000026777887,0.00011426306,0.00007135978,0.019586999,0.0014184294,0.00016129941,0.0023400625,0.000018736993],"about_ca_topic_score_codex":0.009565315,"about_ca_topic_score_gemma":0.008190752,"teacher_disagreement_score":0.009565315,"about_ca_system_score_codex":0.0005347902,"about_ca_system_score_gemma":0.00016356699,"threshold_uncertainty_score":0.019019306},"labels":[],"label_agreement":null},{"id":"W4220845895","doi":"10.3847/1538-4357/ac4744","title":"Two New Black Widow Millisecond Pulsars in M28","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Millisecond pulsar; Pulsar; Physics; Globular cluster; Astrophysics; Astronomy; Stars; X-ray pulsar; Telescope; Cluster (spacecraft)","score_opus":0.01316765420050628,"score_gpt":0.3116838284109133,"score_spread":0.298516174210407,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220845895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99930406,0.00006523265,0.00010533816,0.000056894165,0.000009265856,0.0000050074764,0.000058760834,0.000007420273,0.00038783462],"genre_scores_gemma":[0.99870896,0.00005381478,0.0004664028,0.00005464316,0.000016496626,0.0000060676302,0.00018894448,0.0000040169275,0.0005005647],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998684,0.000008467432,0.000006975543,0.000039918534,0.000040304352,0.000035898065],"domain_scores_gemma":[0.9995895,0.00004142303,0.00009138772,0.000055354496,0.00003963212,0.00018262917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017515052,0.00020720907,0.00026534335,0.0009466611,0.0007232302,0.00051647506,0.00042899372,0.00053683994,0.0011452181],"category_scores_gemma":[0.0005824235,0.00017160656,0.00016770695,0.0005730412,0.00043050415,0.0003612071,0.0013229866,0.0005115806,0.00037472544],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005323114,0.00015402639,0.91736865,0.00003957276,0.000044090266,0.010996046,0.0025649387,0.00018003731,0.04244641,0.0008388678,0.0011025395,0.023732621],"study_design_scores_gemma":[0.0000825127,0.000663173,0.9603526,0.000020780826,0.000033066877,0.012950622,0.001270701,0.0008485533,0.00761306,0.0011913377,0.014943708,0.000029914087],"about_ca_topic_score_codex":0.0016232985,"about_ca_topic_score_gemma":0.003104091,"teacher_disagreement_score":0.0016232985,"about_ca_system_score_codex":0.00031390542,"about_ca_system_score_gemma":0.00014338613,"threshold_uncertainty_score":0.0038311481},"labels":[],"label_agreement":null},{"id":"W4220848861","doi":"10.3847/1538-4357/ac3240","title":"Toward a Better Understanding of Cosmic Chronometers: Stellar Population Properties of Passive Galaxies at Intermediate Redshift","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Ministero dell’Istruzione, dell’Università e della Ricerca","keywords":"Physics; Astrophysics; Redshift; Galaxy; Population; Stellar population; Star formation; Cosmic time; COSMIC cancer database; Photometric redshift","score_opus":0.024380949785410475,"score_gpt":0.2104290299077829,"score_spread":0.18604808012237242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220848861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9581773,0.0005083992,0.025357898,0.00023002272,0.00002009479,0.000023274579,0.009627676,0.0012205835,0.004834746],"genre_scores_gemma":[0.98592156,0.000103945735,0.007492027,0.00006168832,0.00002601547,0.000019126086,0.0059198993,0.00016802753,0.00028771203],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972886,0.000058649963,0.000013858436,0.000115615854,0.00004902753,0.000034032873],"domain_scores_gemma":[0.9968054,0.00081397186,0.0011910673,0.0005331422,0.0003384004,0.00031803967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016268634,0.00045547087,0.00030825724,0.0030494784,0.00020701812,0.0014053013,0.00058058155,0.00034045274,0.0020267477],"category_scores_gemma":[0.0038045195,0.00027165274,0.00041632698,0.0016850486,0.00030428328,0.001019246,0.00070072414,0.0005197573,0.00075895456],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000053861757,0.000033599117,0.9725159,0.0000623753,0.000113752074,0.000024738902,0.00021278231,0.0034175941,0.006357707,0.0015201378,0.0009481261,0.014739563],"study_design_scores_gemma":[0.000006127401,0.000021545795,0.9815238,0.000024126073,0.0000240352,0.00004430187,0.00005962116,0.013682359,0.0015767963,0.00097385375,0.0020485925,0.000014807121],"about_ca_topic_score_codex":0.0041637523,"about_ca_topic_score_gemma":0.0052831303,"teacher_disagreement_score":0.0041637523,"about_ca_system_score_codex":0.00029363896,"about_ca_system_score_gemma":0.00022438001,"threshold_uncertainty_score":0.008603811},"labels":[],"label_agreement":null},{"id":"W4220862543","doi":"10.3847/1538-4357/ac5628","title":"Embedded Young Massive Star Clusters in the Antennae Merger","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Institutes of Natural Sciences; National Aeronautics and Space Administration; Canada Research Chairs; Associated Universities; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Molecular cloud; Star cluster; Star formation; Galaxy; Stars; Cluster (spacecraft); Virial theorem; Astronomy","score_opus":0.009883304803258303,"score_gpt":0.2358184904019273,"score_spread":0.22593518559866899,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220862543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994717,0.000043148146,0.00015540319,0.000011502765,0.0000010295159,0.0000014980566,0.000045842742,0.000005494499,0.00026432757],"genre_scores_gemma":[0.99977666,0.000010686211,0.00008013413,0.0000034531665,0.0000029424182,7.127541e-7,0.000074863165,8.884481e-7,0.000049626422],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998901,0.000014108852,0.000005620501,0.000033795386,0.000026218084,0.000030148121],"domain_scores_gemma":[0.99944097,0.000071724964,0.00023756974,0.00003667863,0.000050938626,0.00016204263],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002035131,0.00014722455,0.00023310161,0.0007741842,0.00053743616,0.00062627957,0.0002051154,0.00021981249,0.000842379],"category_scores_gemma":[0.00047407052,0.00014431794,0.00012602999,0.0006848792,0.00041657788,0.0002890564,0.0006677232,0.00022668343,0.0001867797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014734697,0.000025333922,0.98439527,0.000011461673,0.000037159378,0.00067035516,0.00024251718,0.0010463753,0.010349552,0.00042052777,0.00020169506,0.0024523158],"study_design_scores_gemma":[0.0000067168276,0.000025178271,0.9965288,0.0000018914847,0.00001027379,0.00033638568,0.0001829903,0.0017100808,0.000702043,0.00016591689,0.0003254107,0.000004307116],"about_ca_topic_score_codex":0.0033629173,"about_ca_topic_score_gemma":0.0029923723,"teacher_disagreement_score":0.0033629173,"about_ca_system_score_codex":0.00032954267,"about_ca_system_score_gemma":0.00011881833,"threshold_uncertainty_score":0.0066866875},"labels":[],"label_agreement":null},{"id":"W4220888079","doi":"10.3847/1538-4357/ac3094","title":"Testing the Momentum-driven Supernova Feedback Paradigm in M31","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Supernova; Momentum (technical analysis); Galaxy; Interstellar medium; Angular momentum; Turbulence; Velocity dispersion; Molecular cloud; Stars; Classical mechanics; Mechanics","score_opus":0.015064425157243478,"score_gpt":0.2156828632821777,"score_spread":0.2006184381249342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220888079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996842,0.000006451365,0.00017467634,0.000004820269,3.9227825e-7,0.0000016055164,0.000016223958,0.0000031714433,0.00010848404],"genre_scores_gemma":[0.9998274,0.0000031288776,0.0001233192,0.0000019554896,4.4862867e-7,0.0000010614823,0.000019150655,6.325086e-7,0.000022857817],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998425,0.000045331693,0.000009799544,0.000043710214,0.000024406014,0.000034229644],"domain_scores_gemma":[0.99897254,0.00038636872,0.00022704361,0.0001359713,0.00008687163,0.00019125827],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068103516,0.0003198482,0.00021681264,0.00035690275,0.00033979528,0.00033792513,0.00045905134,0.00034306364,0.00070994167],"category_scores_gemma":[0.0015343217,0.00013101155,0.00029046918,0.00024205874,0.00048941653,0.00044617007,0.00057250645,0.00018171882,0.00013606099],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087445974,0.00039204344,0.82812697,0.000061006653,0.00013308885,0.0006649013,0.00056310603,0.055194456,0.10260038,0.0026845655,0.00015904181,0.008546006],"study_design_scores_gemma":[0.000057241512,0.00094630034,0.8433561,0.000012095957,0.000049034294,0.00029821164,0.0005003838,0.1336045,0.018841129,0.0019161594,0.00038860616,0.000030292787],"about_ca_topic_score_codex":0.008424278,"about_ca_topic_score_gemma":0.0057145567,"teacher_disagreement_score":0.008424278,"about_ca_system_score_codex":0.00056667504,"about_ca_system_score_gemma":0.00028730158,"threshold_uncertainty_score":0.016750515},"labels":[],"label_agreement":null},{"id":"W4220930995","doi":"10.3847/1538-4357/ac4497","title":"On the Spectral Evolution of Hot White Dwarf Stars. II. Time-dependent Simulations of Element Transport in Evolving White Dwarfs with STELUM","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"White dwarf; Physics; Astrophysics; Stellar evolution; Black dwarf; Blue dwarf; Effective temperature; Stellar classification; Helium; Stars; Atomic physics","score_opus":0.007219997885983607,"score_gpt":0.202986108041084,"score_spread":0.1957661101551004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220930995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897085,0.000117853684,0.0039202035,0.00020769972,0.000020852287,0.00003122118,0.00035598304,0.00017857154,0.0054591037],"genre_scores_gemma":[0.9939167,0.000071526265,0.004490646,0.00007357181,0.000010008042,0.000036580812,0.00043926464,0.000059848382,0.0009020456],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998605,0.000042894255,0.0000055172554,0.000015424284,0.00003012131,0.00004550442],"domain_scores_gemma":[0.99873394,0.0008273578,0.00013065134,0.0000612208,0.00013971412,0.00010719417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00064385124,0.0005354303,0.00058167044,0.0006259182,0.00069891947,0.00063371373,0.0010384545,0.0010799103,0.0012428055],"category_scores_gemma":[0.0026171084,0.00026664764,0.0006090266,0.0005184292,0.0008538785,0.00044678253,0.00068402593,0.0007366443,0.00017434655],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000106537685,0.0001007598,0.008924534,0.000040688625,0.000029307703,0.00012227404,0.0001019203,0.9833799,0.0019991712,0.0027446146,0.00043664937,0.0020137061],"study_design_scores_gemma":[0.00002153239,0.0000249542,0.0012467591,0.000005263857,0.0000032783616,0.000005950641,0.000030462154,0.9977647,0.00041338205,0.00028759372,0.00019242907,0.0000036492704],"about_ca_topic_score_codex":0.02479187,"about_ca_topic_score_gemma":0.017651564,"teacher_disagreement_score":0.02479187,"about_ca_system_score_codex":0.001417838,"about_ca_system_score_gemma":0.0008874485,"threshold_uncertainty_score":0.049295127},"labels":[],"label_agreement":null},{"id":"W4220935009","doi":"10.3847/1538-4357/ac5021","title":"Exploring the Sgr–Milky Way–disk Interaction Using High-resolution N-body Simulations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Physics; Astrophysics; Asymmetry; Galaxy; Dwarf galaxy; Halo; Supermassive black hole; Astronomy; Perturbation (astronomy)","score_opus":0.05309329971822122,"score_gpt":0.26455668504344204,"score_spread":0.21146338532522083,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220935009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9911322,0.00012760414,0.002105035,0.00031204772,0.00002876705,0.00003236801,0.00055959856,0.00014311213,0.005559299],"genre_scores_gemma":[0.9955128,0.00006443402,0.00300516,0.00012264462,0.000016834958,0.00003964247,0.00070516416,0.00005049132,0.0004828166],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997608,0.00008461586,0.000011930262,0.000042011507,0.000040575134,0.000060106202],"domain_scores_gemma":[0.9969309,0.0021761123,0.0002033087,0.00016650336,0.000254028,0.00026914023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00086290785,0.00066554314,0.0010179373,0.00077713566,0.0010132857,0.0012015526,0.0018833186,0.0017584381,0.0024214056],"category_scores_gemma":[0.0048494535,0.0004690657,0.0010386424,0.00072597223,0.0010399608,0.0008816053,0.00087652274,0.0013924058,0.00021268529],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014247121,0.0001981557,0.01381454,0.00003584878,0.00012969182,0.00012010328,0.000102179496,0.98132193,0.00063822063,0.0018984743,0.0005682323,0.0010301489],"study_design_scores_gemma":[0.000066796165,0.000042614363,0.002213874,0.0000068748286,0.000019407118,0.000011071422,0.00006169763,0.9966041,0.00016234619,0.00053900236,0.0002638058,0.000008330221],"about_ca_topic_score_codex":0.04589033,"about_ca_topic_score_gemma":0.03200137,"teacher_disagreement_score":0.04589033,"about_ca_system_score_codex":0.001500455,"about_ca_system_score_gemma":0.0013502943,"threshold_uncertainty_score":0.091246426},"labels":[],"label_agreement":null},{"id":"W4220954547","doi":"10.3847/1538-4357/ac50b6","title":"A Giant Shell of Ionized Gas Discovered near M82 with the Dragonfly Spectral Line Mapper Pathfinder","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics","score_opus":0.005710322342775229,"score_gpt":0.19082818047474737,"score_spread":0.18511785813197212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4220954547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9923051,0.00011167023,0.00165149,0.00014454123,0.000010368887,0.000018469651,0.001295471,0.00036216681,0.004100574],"genre_scores_gemma":[0.9914773,0.000042786163,0.0056384476,0.00010684119,0.000016637618,0.000012562686,0.0011871674,0.000037226335,0.0014810038],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999496,0.0000024599253,0.0000010515148,0.000019124085,0.000013400167,0.0000144373935],"domain_scores_gemma":[0.99988866,0.000016920168,0.000019557114,0.00001958397,0.000015050073,0.00004027036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008782149,0.00015446542,0.00011522187,0.00068116985,0.0002617979,0.00018903289,0.00023975749,0.0002027413,0.0018238522],"category_scores_gemma":[0.00014213065,0.00011616012,0.00008547698,0.00026264042,0.00011900928,0.00027698747,0.0004121523,0.00014879249,0.00037865073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00080508995,0.00014497817,0.4519164,0.00011639252,0.00009639373,0.0080107255,0.0013098705,0.0024297982,0.40858287,0.0015782571,0.020433506,0.1045757],"study_design_scores_gemma":[0.000050073886,0.00016135834,0.92700356,0.00004542167,0.000034878154,0.0033731645,0.0003747928,0.008384839,0.032212447,0.00046239005,0.02786159,0.000035477813],"about_ca_topic_score_codex":0.003014065,"about_ca_topic_score_gemma":0.009017284,"teacher_disagreement_score":0.003014065,"about_ca_system_score_codex":0.00022034589,"about_ca_system_score_gemma":0.00008250361,"threshold_uncertainty_score":0.00610137},"labels":[],"label_agreement":null},{"id":"W4221010015","doi":"10.3847/1538-4357/ac49e0","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): A Hot Corino Survey toward Protostellar Cores in the Orion Cloud","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Japan Society for the Promotion of Science; Agencia Nacional de Investigación y Desarrollo; National Research Foundation of Korea; Chinese Academy of Sciences; Ministry of Science and Technology, Taiwan; National Natural Science Foundation of China","keywords":"Astrophysics; Physics; Molecular cloud; Luminosity; Planck; Astronomy; Millimeter; Interstellar medium; Submillimeter Array; Star formation; Stars; Galaxy","score_opus":0.03513457963589228,"score_gpt":0.26607825538860497,"score_spread":0.23094367575271268,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221010015","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99900717,0.00009484187,0.000048440208,0.0000098000155,0.0000011397501,0.00000874967,0.0004690352,0.000006371764,0.0003544289],"genre_scores_gemma":[0.9985676,0.00007642675,0.00019873584,0.000014284617,0.000007139757,0.000009589954,0.0008451853,0.0000036293743,0.0002773309],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984074,0.00002045927,0.000007830654,0.00004931505,0.00003736313,0.00004423499],"domain_scores_gemma":[0.99952567,0.000041449865,0.00014224992,0.00004248311,0.00006784588,0.00018038412],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024544692,0.00020413344,0.00016292444,0.0016530032,0.00039128217,0.00031924044,0.00024890125,0.00013657832,0.0009247881],"category_scores_gemma":[0.00035863198,0.000086927736,0.00013847904,0.00076793134,0.00016221973,0.00017702884,0.00055228727,0.000099878205,0.00018349216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005364174,0.00002091657,0.98583835,0.000015874773,0.000030140318,0.000095377545,0.00022655289,0.000050559072,0.009579935,0.000051404997,0.00022779603,0.003809376],"study_design_scores_gemma":[0.0000016267383,0.000012974529,0.9991365,0.0000016021353,0.000004190517,0.00004098203,0.00008552058,0.00007505227,0.0003162613,0.0000045659995,0.0003197437,9.081082e-7],"about_ca_topic_score_codex":0.016071018,"about_ca_topic_score_gemma":0.01971612,"teacher_disagreement_score":0.016071018,"about_ca_system_score_codex":0.0003162828,"about_ca_system_score_gemma":0.00024628075,"threshold_uncertainty_score":0.031954944},"labels":[],"label_agreement":null},{"id":"W4221033192","doi":"10.3847/1538-4357/ac5620","title":"SDSS-IV MaNGA: Understanding Ionized Gas Turbulence Using Integral Field Spectroscopy of 4500 Star-forming Disk Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Velocity dispersion; Sigma; Galaxy; Star formation; Stars; Spectroscopy; Ionization; Astronomy","score_opus":0.018644000092626883,"score_gpt":0.23947027777440788,"score_spread":0.220826277681781,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221033192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99703205,0.00014442703,0.0006994437,0.000063652435,0.0000032157827,0.000017527555,0.0012005941,0.00012520008,0.0007138276],"genre_scores_gemma":[0.99664116,0.000047507034,0.0018419537,0.000028253648,0.0000102774875,0.000010035169,0.0012644408,0.000018361152,0.00013791116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998468,0.00003150901,0.000009472005,0.000050757586,0.000027433027,0.000034065462],"domain_scores_gemma":[0.99940467,0.00010830425,0.00015902106,0.000083272025,0.00006260188,0.000182142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00083255535,0.00031060103,0.00028969813,0.0015477533,0.00033662032,0.0006997138,0.00038401157,0.00021079944,0.00059821876],"category_scores_gemma":[0.0009620493,0.00025063992,0.00041164475,0.0007478886,0.00020480585,0.00052919216,0.00047051575,0.0001878388,0.0002332864],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007451277,0.00007830169,0.98191833,0.000019715206,0.00007569614,0.00007949556,0.00021862624,0.001745574,0.007663741,0.00027574395,0.0006340027,0.0072163315],"study_design_scores_gemma":[0.00000810733,0.00001909391,0.9896326,0.0000055985543,0.000011654777,0.000024879746,0.00009635781,0.009274872,0.00040081644,0.00013511394,0.00038426524,0.000006577248],"about_ca_topic_score_codex":0.016673943,"about_ca_topic_score_gemma":0.024416273,"teacher_disagreement_score":0.016673943,"about_ca_system_score_codex":0.0005931858,"about_ca_system_score_gemma":0.0002773212,"threshold_uncertainty_score":0.033153772},"labels":[],"label_agreement":null},{"id":"W4221077745","doi":"10.3847/1538-4357/ac460b","title":"Probing the Local Interstellar Medium with Scintillometry of the Bright Pulsar B1133 + 16","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; RES’EAU-WaterNET; University of Central Florida; National Science Foundation","keywords":"Physics; Scintillation; Scattering; Interstellar medium; Pulsar; Population; Astrophysics; Line-of-sight; Optics","score_opus":0.007524697675381566,"score_gpt":0.26137360815997507,"score_spread":0.2538489104845935,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221077745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984434,0.00003195711,0.00090788386,0.000008323118,0.0000011161907,0.00000205349,0.00014213845,0.000029204926,0.00043391576],"genre_scores_gemma":[0.9990381,0.000024832045,0.00051536283,0.000003071357,0.000001161502,0.0000025361073,0.0003049587,0.00001675519,0.00009327175],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999484,0.0000049431133,0.0000019486126,0.000020570493,0.000012863666,0.000011340794],"domain_scores_gemma":[0.999881,0.000025847907,0.000045667774,0.000016464342,0.0000147045785,0.000016284419],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019398126,0.0001828932,0.0002701954,0.0005469293,0.00025511658,0.00044789785,0.00021802742,0.00016550564,0.00071933004],"category_scores_gemma":[0.0002666423,0.00017269551,0.00029920074,0.0006065553,0.00020668343,0.0002312984,0.0003091776,0.00026546835,0.00016304161],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029180833,0.0000652638,0.6364002,0.000056509234,0.00014774551,0.00020920855,0.00022525094,0.020555545,0.32735208,0.00042538636,0.00019414409,0.014076856],"study_design_scores_gemma":[0.000015969075,0.00007957635,0.9396269,0.000007839716,0.00004912474,0.00010014663,0.00012744588,0.039021518,0.019719869,0.00020766325,0.0010260136,0.000017998282],"about_ca_topic_score_codex":0.007936587,"about_ca_topic_score_gemma":0.013893308,"teacher_disagreement_score":0.007936587,"about_ca_system_score_codex":0.00040256025,"about_ca_system_score_gemma":0.00016854808,"threshold_uncertainty_score":0.015780807},"labels":[],"label_agreement":null},{"id":"W4221091829","doi":"10.3847/1538-4357/ac53ac","title":"Dust Dynamics in Transitional Disks: Clumping and Disk Recession","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Rotational symmetry; Mechanics; Drag; Radiation; Physics; Dynamics (music); Instability; Enhanced Data Rates for GSM Evolution; Radiation pressure; Flow (mathematics); Astrophysics; Optics","score_opus":0.007833835324291384,"score_gpt":0.2347018362716992,"score_spread":0.2268680009474078,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221091829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99767154,0.000064064625,0.0011744903,0.000054151897,0.0000067607193,0.000005469111,0.000032502834,0.000031479707,0.0009594343],"genre_scores_gemma":[0.99967015,0.00001881652,0.0001852802,0.0000063737493,0.0000016049336,0.0000021268017,0.000013700631,0.0000048731054,0.000097077056],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999502,0.000006377402,0.0000026709592,0.0000109705925,0.0000078868925,0.00002204607],"domain_scores_gemma":[0.99978083,0.00004840122,0.000046746205,0.000022894234,0.000021028412,0.00008013484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001137928,0.000260345,0.000348091,0.0002494429,0.00042059927,0.00080366875,0.00061555253,0.00044934778,0.0011638581],"category_scores_gemma":[0.000763802,0.00021477611,0.00034577333,0.00016647442,0.00056377635,0.0005810144,0.0007093036,0.00045364775,0.0001245753],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016647899,0.00067501876,0.16963747,0.00025671476,0.00024063785,0.0031061892,0.0009273386,0.60517216,0.19540909,0.009144172,0.001438148,0.012328294],"study_design_scores_gemma":[0.00017089384,0.00031678926,0.06330602,0.000017871362,0.000034242712,0.0003142242,0.00040405366,0.92354536,0.008454508,0.0024959666,0.0009000291,0.000039968247],"about_ca_topic_score_codex":0.004732266,"about_ca_topic_score_gemma":0.0016950978,"teacher_disagreement_score":0.004732266,"about_ca_system_score_codex":0.00048217064,"about_ca_system_score_gemma":0.0002367912,"threshold_uncertainty_score":0.009409428},"labels":[],"label_agreement":null},{"id":"W4221122945","doi":"10.3847/1538-4357/ac4780","title":"A Carbon/Oxygen-dominated Atmosphere Days after Explosion for the “Super-Chandrasekhar” Type Ia SN 2020esm","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of Illinois at Urbana-Champaign; Agencia Nacional de Investigación y Desarrollo; Max-Planck-Gesellschaft; Queen's University; Gordon and Betty Moore Foundation; Queen's University Belfast; Max-Planck-Institut für Astronomie; University of Edinburgh; Durham University; Northwestern University; National Central University; Villum Fonden; Los Alamos National Laboratory; Johns Hopkins University; Nuclear Safety and Security Commission; Heising-Simons Foundation; Australian Research Council; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; W. M. Keck Foundation; National Centre for Supercomputing Applications; Eötvös Loránd Tudományegyetem; European Commission; California Institute of Technology; National Aeronautics and Space Administration; David and Lucile Packard Foundation; Smithsonian Institution; National Science Foundation","keywords":"Physics; Supernova; Astrophysics; White dwarf; Chandrasekhar limit; Light curve; Spectral line; Ejecta; Stellar evolution; Stars; Astronomy","score_opus":0.010476785890499163,"score_gpt":0.2297675793646417,"score_spread":0.21929079347414254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221122945","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992391,0.000035294895,0.00007276151,0.00000938814,0.0000029013704,0.000001265038,0.00012596532,0.000009875884,0.0005035051],"genre_scores_gemma":[0.9992513,0.000017055974,0.00013441367,0.0000090958865,0.0000034714456,0.0000011452372,0.00040194503,0.000003285138,0.0001781932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999726,0.0000017259346,0.00000168541,0.000008912801,0.000006778277,0.000008282092],"domain_scores_gemma":[0.99989986,0.0000073760502,0.000032561515,0.0000076964625,0.000013087915,0.00003936218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000104343395,0.00015699583,0.00010819721,0.00032985417,0.00021946571,0.0002644435,0.00012499176,0.00014249815,0.0005981834],"category_scores_gemma":[0.00014959785,0.00008505556,0.00012918968,0.00014731949,0.00011440414,0.00012326991,0.00020051317,0.00024271278,0.00016349588],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005726762,0.00012495895,0.90485156,0.00002817636,0.000051222538,0.00088287744,0.00015272491,0.00044939984,0.084668115,0.00040843603,0.00053908466,0.0072706747],"study_design_scores_gemma":[0.0000047458216,0.000082914645,0.9943792,0.0000026755015,0.000008408974,0.00040747208,0.00006965201,0.0009484798,0.0033784776,0.000087991124,0.0006259254,0.0000040001037],"about_ca_topic_score_codex":0.0019190793,"about_ca_topic_score_gemma":0.0040469375,"teacher_disagreement_score":0.0019190793,"about_ca_system_score_codex":0.00015845495,"about_ca_system_score_gemma":0.00008625197,"threshold_uncertainty_score":0.0038158298},"labels":[],"label_agreement":null},{"id":"W4221138269","doi":"10.3847/1538-4357/ac74c0","title":"4–8 GHz Fourier-domain Searches for Galactic Center Pulsars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Precursory Research for Embryonic Science and Technology; Breakthrough Prize Foundation; National Science Foundation","keywords":"Pulsar; Physics; Astrophysics; Magnetar; Millisecond pulsar; Galaxy; Galactic Center; Astronomy; Supermassive black hole; Neutron star; Green Bank Telescope; Pulsar planet; Binary pulsar; Interstellar medium; Population; X-ray pulsar","score_opus":0.021696308535294796,"score_gpt":0.32624646803419566,"score_spread":0.30455015949890085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221138269","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99583685,0.00010309795,0.0019192673,0.00006370243,0.000005391858,0.000006066399,0.00038268729,0.00008700739,0.0015959939],"genre_scores_gemma":[0.9957283,0.00004669635,0.0031962697,0.00002195659,0.000019902942,0.0000063676866,0.00051007076,0.000008118294,0.00046230757],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999424,0.000009386097,0.000002789023,0.000017044265,0.000012563077,0.000015939908],"domain_scores_gemma":[0.9996761,0.000093545445,0.0001158075,0.000037791957,0.00003305484,0.000043703603],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017584144,0.00012860757,0.00011152582,0.0010276453,0.00016707313,0.00027248904,0.00015966235,0.00016534663,0.0017126929],"category_scores_gemma":[0.0004271063,0.00007527182,0.00007505807,0.00045228848,0.000108064196,0.00015874804,0.00022684515,0.00015166569,0.00027536444],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030668947,0.00011288826,0.7494522,0.000051947787,0.00006708185,0.0004256399,0.00024503542,0.0010339592,0.18902703,0.000650916,0.0013769239,0.057249624],"study_design_scores_gemma":[0.000011318974,0.000087946246,0.98656183,0.0000067977517,0.000024906578,0.00048013293,0.00010205398,0.0022747414,0.00781343,0.00033574057,0.0022945434,0.0000065155928],"about_ca_topic_score_codex":0.0005523212,"about_ca_topic_score_gemma":0.00089326897,"teacher_disagreement_score":0.0017126929,"about_ca_system_score_codex":0.00009137481,"about_ca_system_score_gemma":0.000057965375,"threshold_uncertainty_score":0.0057294965},"labels":[],"label_agreement":null},{"id":"W4221139988","doi":"10.3847/1538-4357/ac61dd","title":"An Assessment of the In Situ Growth of the Intracluster Light in the High-redshift Galaxy Cluster SpARCS1049+56","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; York University; Université de Montréal; McGill University","funders":"","keywords":"Physics; Astrophysics; Star formation; Redshift; Galaxy; Stellar mass; Cluster (spacecraft); Intracluster medium; Stars; Galaxy cluster; Astronomy","score_opus":0.005564364403106649,"score_gpt":0.22956816378248082,"score_spread":0.22400379937937417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221139988","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995161,0.000023336994,0.000075072974,0.0000059248255,0.0000011278476,0.0000011329369,0.00013938473,0.000009441965,0.00022850842],"genre_scores_gemma":[0.99933004,0.000013987053,0.00015012267,0.0000041573985,0.000002009938,0.0000012326278,0.00036240302,0.00000515945,0.00013096577],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988616,0.000009586669,0.0000046264295,0.000042008436,0.000030641462,0.0000269541],"domain_scores_gemma":[0.99952614,0.000064998225,0.000107573236,0.00005754829,0.00014034731,0.00010340305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025313828,0.00015546533,0.0001811538,0.0008318158,0.00030202256,0.0004673071,0.0002407824,0.00021667975,0.0006877702],"category_scores_gemma":[0.00042251917,0.00014547879,0.00018163689,0.00045621453,0.0002557032,0.00023161132,0.0003391954,0.00016498897,0.0002329219],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009586545,0.00002736426,0.95628244,0.000017527092,0.000058451456,0.00010550672,0.00025704858,0.0010950742,0.037714846,0.00007178498,0.00017675068,0.0040973723],"study_design_scores_gemma":[0.0000012137348,0.000019296673,0.99730635,0.0000010122387,0.000010017276,0.000034102242,0.00007956785,0.0009265818,0.0014675236,0.00000913836,0.00014310486,0.0000020908012],"about_ca_topic_score_codex":0.010591126,"about_ca_topic_score_gemma":0.021638222,"teacher_disagreement_score":0.010591126,"about_ca_system_score_codex":0.0003702041,"about_ca_system_score_gemma":0.00012167779,"threshold_uncertainty_score":0.021058917},"labels":[],"label_agreement":null},{"id":"W4221140911","doi":"10.3847/1538-4357/ac63aa","title":"A Radio, Optical, UV, and X-Ray View of the Enigmatic Changing-look Active Galactic Nucleus 1ES 1927+654 from Its Pre- to Postflare States","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Goddard Space Flight Center; Ministerio de Ciencia e Innovación; Israel Science Foundation; European Commission; Alan Turing Institute; Agencia Estatal de Investigación; National Aeronautics and Space Administration","keywords":"Physics; Flare; Astrophysics; Light curve; Observatory; Astronomy; Very-long-baseline interferometry; Active galactic nucleus; Emission spectrum; Galaxy; Spectral line","score_opus":0.009063452087236877,"score_gpt":0.2224877935920847,"score_spread":0.21342434150484782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221140911","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99408466,0.0003013256,0.00012587539,0.00011704579,0.0000126730165,0.000006101992,0.0011132002,0.00003777944,0.004201328],"genre_scores_gemma":[0.99623257,0.00015908973,0.00034234926,0.000045911263,0.000024155772,0.000004488806,0.0016173156,0.000009568151,0.0015644927],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995637,0.0000040212312,0.0000021251033,0.000012203936,0.000010559783,0.00001461881],"domain_scores_gemma":[0.9998373,0.000011855137,0.000054066684,0.000013224049,0.000036657144,0.000046751346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012943753,0.00012843979,0.00008471566,0.0012501517,0.00031367803,0.0004874864,0.0001564004,0.00024703448,0.0016685199],"category_scores_gemma":[0.00017629423,0.00008834621,0.00012404531,0.0006217767,0.00019522352,0.00022626884,0.00043682964,0.00027808294,0.0003590877],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022413066,0.00010922579,0.9420201,0.000056055167,0.00005426658,0.0020913472,0.0012103126,0.0006944512,0.02274033,0.00037315305,0.0035308085,0.026895741],"study_design_scores_gemma":[0.0000012596465,0.00002103997,0.9975352,0.000005453469,0.000005458443,0.00020618258,0.0001922568,0.00009974723,0.00022050741,0.000029391145,0.0016810809,0.0000023109505],"about_ca_topic_score_codex":0.010187178,"about_ca_topic_score_gemma":0.021053502,"teacher_disagreement_score":0.010187178,"about_ca_system_score_codex":0.00033826276,"about_ca_system_score_gemma":0.0000985533,"threshold_uncertainty_score":0.020255744},"labels":[],"label_agreement":null},{"id":"W4221141271","doi":"10.3847/1538-4357/ac67a8","title":"A Spectroscopic View of the JWST/GTO Strong Lensing Cluster A1489","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; University of Oxford; York University; Dipartimenti di Eccellenza; Leibniz-Gemeinschaft; University of Notre Dame; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ministero dell’Istruzione, dell’Università e della Ricerca; Carnegie Mellon University; Universidad Nacional Autónoma de México; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Max-Planck-Institut für Astrophysik","keywords":"Physics; Velocity dispersion; Astrophysics; Cluster (spacecraft); Redshift; Photometry (optics); Weak gravitational lensing; Strong gravitational lensing; Dispersion (optics); Galaxy; Stars; Optics","score_opus":0.008675271332220227,"score_gpt":0.21860085977300234,"score_spread":0.2099255884407821,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221141271","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970867,0.000039836035,0.00015479334,0.00004113072,0.0000018875292,0.0000019273878,0.00020892864,0.000011860999,0.0024530105],"genre_scores_gemma":[0.9993525,0.00001620401,0.00020464354,0.000011000767,0.0000057451084,0.000001465776,0.00017249155,0.0000024861533,0.00023333365],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997175,0.0000022764466,0.000001421608,0.000008972731,0.000008216349,0.0000073395927],"domain_scores_gemma":[0.9998524,0.000012848394,0.000051346986,0.000011964683,0.000021728334,0.000049709855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000041020034,0.00009880455,0.000091632915,0.0013197208,0.0003626734,0.00028507836,0.00017940288,0.00015364603,0.0015680642],"category_scores_gemma":[0.0001841619,0.000079595855,0.00006819189,0.00044718842,0.0001656801,0.00020857599,0.00037621052,0.00011558512,0.00023064479],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036895365,0.00008896448,0.73768014,0.000050899453,0.000035025547,0.0016295603,0.0010190635,0.0014982913,0.2301056,0.0039476696,0.0019737952,0.021602098],"study_design_scores_gemma":[0.000008286091,0.000041699688,0.9936738,0.000007882927,0.0000075209086,0.0005515123,0.00027727868,0.0016126992,0.0016047329,0.0005778838,0.0016317123,0.000004905345],"about_ca_topic_score_codex":0.0041409275,"about_ca_topic_score_gemma":0.007041269,"teacher_disagreement_score":0.0041409275,"about_ca_system_score_codex":0.00021901188,"about_ca_system_score_gemma":0.00007542674,"threshold_uncertainty_score":0.008233607},"labels":[],"label_agreement":null},{"id":"W4221145789","doi":"10.3847/1538-4357/ac62cd","title":"Detection of a Superluminous Spiral Galaxy in the Heart of a Massive Galaxy Cluster","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Smithsonian Institution; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Astrophysics; Brightest cluster galaxy; Galaxy cluster; Elliptical galaxy; Interacting galaxy; Lenticular galaxy; Cluster (spacecraft); Galaxy; Astronomy","score_opus":0.007523086721670098,"score_gpt":0.20863587990336901,"score_spread":0.20111279318169892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221145789","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99862504,0.000045917182,0.00028638722,0.000020502559,0.0000021055412,0.0000030306874,0.00008645362,0.00004002192,0.0008905078],"genre_scores_gemma":[0.9993431,0.000011628094,0.00024075771,0.000012595291,0.000002530891,0.0000015401072,0.00013240961,0.000004410144,0.00025117345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991727,0.000007128996,0.000003421254,0.000029029563,0.000018050754,0.000025050813],"domain_scores_gemma":[0.9996531,0.00002953044,0.00009270255,0.000038726554,0.00004491571,0.00014095457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013492198,0.00012424929,0.00014027907,0.000692953,0.00030836923,0.00038104824,0.00020380496,0.00017474832,0.0023912098],"category_scores_gemma":[0.0002895951,0.00010412682,0.00008114828,0.0004319886,0.00028901617,0.00013865822,0.00040562925,0.00012816647,0.0004897448],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001412325,0.000034047127,0.9449874,0.000016649787,0.00002339324,0.00045628948,0.00036378202,0.00015084285,0.046748675,0.00039877792,0.0005818376,0.006097056],"study_design_scores_gemma":[0.0000043884465,0.00003792175,0.9953904,0.0000038011055,0.000011605676,0.00035102785,0.00013594166,0.00031218713,0.0027441243,0.00009195001,0.0009119278,0.0000046068308],"about_ca_topic_score_codex":0.003019027,"about_ca_topic_score_gemma":0.004037324,"teacher_disagreement_score":0.003019027,"about_ca_system_score_codex":0.0002139616,"about_ca_system_score_gemma":0.00010296064,"threshold_uncertainty_score":0.00799942},"labels":[],"label_agreement":null},{"id":"W4221146196","doi":"10.3847/1538-4357/ac7155","title":"Discovery of a Cool, Metal-rich Gas Reservoir in the Outskirts of z ≈ 0.5 Clusters","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Quasar; Astrophysics; Redshift; Physics; Cluster (spacecraft); Galaxy; Galaxy cluster; Absorption (acoustics); Equivalent width; Spectral line; Astronomy; Emission spectrum; Optics","score_opus":0.009881853148223289,"score_gpt":0.22089184383372315,"score_spread":0.21100999068549986,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221146196","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99942434,0.000036690122,0.00012835173,0.000007829275,0.0000011204423,0.0000017749552,0.0001145261,0.000013617812,0.0002717359],"genre_scores_gemma":[0.9992506,0.00001733538,0.00014860841,0.000016109896,0.0000034340242,0.0000016645685,0.00037915353,0.0000068474633,0.00017623584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989486,0.000006536487,0.0000030727833,0.00004128674,0.000018349556,0.000035849753],"domain_scores_gemma":[0.99971205,0.000028540302,0.000070870985,0.00002755799,0.000028582956,0.00013227205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014953638,0.00017207583,0.00027878906,0.00089980045,0.0005046069,0.0006912622,0.00035296485,0.00013043504,0.0012171586],"category_scores_gemma":[0.00038675172,0.00017971758,0.00021939415,0.00045562896,0.00034816485,0.00023817399,0.0008384842,0.00020207452,0.00019564111],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022411045,0.0000331541,0.9676137,0.000020885755,0.00004933031,0.00033407396,0.00091140316,0.0003113217,0.02399639,0.0005350959,0.0006625283,0.005308072],"study_design_scores_gemma":[0.0000034616758,0.00002372544,0.99753344,0.0000038684393,0.000013906519,0.000070501395,0.00026107283,0.00048335755,0.00078763824,0.000071373746,0.0007437851,0.000003812258],"about_ca_topic_score_codex":0.008558404,"about_ca_topic_score_gemma":0.012735329,"teacher_disagreement_score":0.008558404,"about_ca_system_score_codex":0.00030794146,"about_ca_system_score_gemma":0.00015363356,"threshold_uncertainty_score":0.017017126},"labels":[],"label_agreement":null},{"id":"W4221146685","doi":"10.3847/1538-4357/ac6ce6","title":"Dynamical Effects of Colliding Outflows in Binary Systems","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Perimeter Institute","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Outflow; Physics; Binary number; Convergence (economics); Orbit (dynamics); Gravitation; Pulsar; Shock (circulatory); Astrophysics; Binary system; Binary star; Collision; Stars; Classical mechanics; Mechanics; Aerospace engineering; Computer science","score_opus":0.006672736813045841,"score_gpt":0.21137423161999574,"score_spread":0.2047014948069499,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221146685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927993,0.00007911329,0.002102801,0.00013533779,0.000025672818,0.000017370203,0.00006416935,0.000048035603,0.0047280667],"genre_scores_gemma":[0.9991146,0.000025129124,0.00046391782,0.00002529375,0.000008411264,0.0000074938575,0.000044597076,0.000013077063,0.00029740616],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998362,0.000040296134,0.000008869141,0.000018373083,0.000032998614,0.00006328316],"domain_scores_gemma":[0.9994766,0.00014443019,0.00011737421,0.00002985774,0.000046450812,0.00018525882],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031676985,0.0003325935,0.0005344065,0.00072277366,0.0013762808,0.0014912382,0.0003868797,0.00073719776,0.0018991649],"category_scores_gemma":[0.0016747151,0.00030682026,0.0004156334,0.00032250935,0.0013490194,0.0008114023,0.0017297479,0.00047807183,0.00014028414],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005350337,0.00027865745,0.038829174,0.000092718765,0.000114967675,0.0022320922,0.0006318554,0.91791373,0.018031018,0.01649387,0.0009369202,0.003910051],"study_design_scores_gemma":[0.00016434738,0.00019804502,0.011062653,0.000021096715,0.00003119207,0.00023723871,0.00035809286,0.9808477,0.0020741674,0.0040793824,0.00088823924,0.000037822254],"about_ca_topic_score_codex":0.005421721,"about_ca_topic_score_gemma":0.002650372,"teacher_disagreement_score":0.005421721,"about_ca_system_score_codex":0.0009440608,"about_ca_system_score_gemma":0.0005050409,"threshold_uncertainty_score":0.0107803345},"labels":[],"label_agreement":null},{"id":"W4221146807","doi":"10.3847/1538-4357/ac7220","title":"Early-time Ultraviolet Spectroscopy and Optical Follow-up Observations of the Type IIP Supernova 2021yja","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; York University; University of California Observatories; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; National Aeronautics and Space Administration; Heising-Simons Foundation; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Astrophysics; Physics; Supernova; Balmer series; Photosphere; Photometry (optics); Ultraviolet; Metallicity; Spectral line; Radiative transfer; Spectroscopy; Emission spectrum; Astronomy; Stars; Optics","score_opus":0.01369559587683063,"score_gpt":0.2256633797605891,"score_spread":0.21196778388375845,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221146807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997999,0.00010065823,0.00020248668,0.000011641107,0.0000047525346,0.000008474329,0.00050819555,0.00002293382,0.0011418039],"genre_scores_gemma":[0.9973459,0.0000488082,0.00046791733,0.000019029612,0.000010335146,0.000009495955,0.0015934933,0.000009802903,0.0004951516],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999542,0.0000030774881,0.0000025700042,0.000011886559,0.000013151388,0.000015067016],"domain_scores_gemma":[0.999681,0.000023447757,0.00007698194,0.000018722638,0.0000588562,0.00014096132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019831728,0.00029711227,0.00023163296,0.0009069618,0.00051548576,0.0004598842,0.00015691607,0.00023644895,0.001065128],"category_scores_gemma":[0.00022190629,0.00015858917,0.0002655496,0.0003856055,0.00012020982,0.000174375,0.00038996618,0.00034561413,0.00033108352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005699135,0.00031365678,0.84059614,0.000082382176,0.00012434296,0.0017196984,0.0003229397,0.0008528085,0.13763231,0.00022160106,0.00090619497,0.016657991],"study_design_scores_gemma":[0.00000520362,0.00009036846,0.996219,0.0000047425065,0.000016890095,0.0003185882,0.00004902286,0.00045081295,0.0022867573,0.000025360938,0.0005286994,0.000004533041],"about_ca_topic_score_codex":0.0027983538,"about_ca_topic_score_gemma":0.0064943708,"teacher_disagreement_score":0.0027983538,"about_ca_system_score_codex":0.00026070914,"about_ca_system_score_gemma":0.00013261383,"threshold_uncertainty_score":0.005564153},"labels":[],"label_agreement":null},{"id":"W4221147984","doi":"10.3847/1538-4357/ac6f5c","title":"EstrellaNueva: An Open-source Software to Study the Interactions and Detection of Neutrinos Emitted by Supernovae","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Laurentian University","funders":"Consejo Nacional de Ciencia y Tecnología; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Fundación Marcos Moshinsky","keywords":"Neutrino; Physics; Supernova; Neutrino detector; Galaxy; Astrophysics; Detector; Cosmic neutrino background; Neutrino astronomy; Neutrino oscillation; Particle physics","score_opus":0.02158017176169764,"score_gpt":0.3074370811900703,"score_spread":0.28585690942837266,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221147984","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.014354678,0.00086579716,0.23533152,0.00021803314,0.00026445667,0.00029942417,0.021478863,0.71682066,0.010366574],"genre_scores_gemma":[0.15648465,0.0019304184,0.43052825,0.0011399161,0.00028179542,0.0026269266,0.095352076,0.28355494,0.028101048],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99941146,0.00007716741,0.00006369765,0.00016240451,0.00020790305,0.00007734556],"domain_scores_gemma":[0.9984068,0.00089069025,0.0001748704,0.00017826824,0.00024642152,0.00010297734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012667611,0.0020714428,0.0012405354,0.0017827742,0.0005460147,0.0015059364,0.0030604952,0.0012469634,0.03400965],"category_scores_gemma":[0.0042034914,0.0011942605,0.0026592873,0.00081863184,0.00053926423,0.0021217987,0.0025826786,0.0020036537,0.013451832],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0026714467,0.000917144,0.027657725,0.007362448,0.0023550892,0.0024679676,0.0010401333,0.07654008,0.042669408,0.041492783,0.43691036,0.35791546],"study_design_scores_gemma":[0.0008593506,0.0002599375,0.012120492,0.0007976994,0.00038544307,0.0013489926,0.00011853504,0.3691773,0.055447128,0.03637266,0.5225094,0.00060312555],"about_ca_topic_score_codex":0.002103436,"about_ca_topic_score_gemma":0.0018409822,"teacher_disagreement_score":0.03400965,"about_ca_system_score_codex":0.0005408242,"about_ca_system_score_gemma":0.0011696289,"threshold_uncertainty_score":0.113773644},"labels":[],"label_agreement":null},{"id":"W4221151524","doi":"10.3847/1538-4357/ac6809","title":"Improved Upper Limit on Degree-scale CMB B-mode Polarization Power from the 670 Square-degree POLARBEAR Survey","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Herzberg Institute of Astrophysics","funders":"Lawrence Berkeley National Laboratory; Comisión Nacional de Investigación Científica y Tecnológica; Natural Sciences and Engineering Research Council of Canada; Dalhousie University; University of California, San Diego; Japan Society for the Promotion of Science; Office of Science; Ministry of Education, Culture, Sports, Science and Technology; High Energy Physics; U.S. Department of Energy","keywords":"Cosmic microwave background; Physics; Planck; Spectral density; Black-body radiation; Polarization (electrochemistry); Sky; Computational physics; Mode (computer interface); Degree (music); Cosmic background radiation; Optics; Astrophysics; Statistics; Mathematics; Anisotropy; Acoustics","score_opus":0.01643835011164822,"score_gpt":0.24780542998149765,"score_spread":0.23136707986984945,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221151524","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94565475,0.0012824459,0.037513588,0.00028446075,0.000055216908,0.000024080626,0.00563195,0.0008004569,0.008752968],"genre_scores_gemma":[0.9881291,0.00024839307,0.007912951,0.000097294855,0.00008090463,0.000020381645,0.003193408,0.00006457259,0.00025296726],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99882656,0.0003920429,0.0000340947,0.00026496634,0.00034631632,0.00013593964],"domain_scores_gemma":[0.99726725,0.0011290379,0.00040214323,0.0005894634,0.00039820024,0.00021397953],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001960299,0.0007041707,0.000374086,0.0019852426,0.0002948663,0.0007177154,0.00046472176,0.00036837644,0.0020743774],"category_scores_gemma":[0.0033001064,0.0003320397,0.00035080378,0.0016840509,0.0003229632,0.00040036903,0.00077465025,0.00046328054,0.00096346514],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001082786,0.00014055663,0.8099326,0.00034538383,0.00039157277,0.000490679,0.00035425313,0.009826018,0.097706296,0.005961364,0.0059475764,0.067820914],"study_design_scores_gemma":[0.000039821287,0.00008851032,0.9551302,0.000053288702,0.000115962444,0.00032073638,0.000092221024,0.013642286,0.016967852,0.0018243508,0.011679313,0.000045376393],"about_ca_topic_score_codex":0.0028708444,"about_ca_topic_score_gemma":0.0029532728,"teacher_disagreement_score":0.0028708444,"about_ca_system_score_codex":0.00029904986,"about_ca_system_score_gemma":0.000138104,"threshold_uncertainty_score":0.010367155},"labels":[],"label_agreement":null},{"id":"W4221151631","doi":"10.3847/1538-4357/ac5ac0","title":"Improving White Dwarfs as Chronometers with Gaia Parallaxes and Spectroscopic Metallicities","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"Los Alamos National Laboratory; Lawrence Berkeley National Laboratory; Australian Astronomical Optics-Macquarie; Australian Research Council; Horizon 2020 Framework Programme; University of Colorado Boulder; Office of Science; Carnegie Institution for Science; Instituto de Astrofísica de Canarias; Max-Planck-Institut für Astrophysik; Leibniz-Institut für Astrophysik Potsdam; National Development and Reform Commission; Eötvös Loránd Tudományegyetem; Natural Sciences and Engineering Research Council of Canada; National Central University; Deutsches Zentrum für Luft- und Raumfahrt; Max-Planck-Gesellschaft; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; York University; Ministério da Ciência, Tecnologia e Inovação; University of Edinburgh; Queen's University; Deutsche Forschungsgemeinschaft; Chinese Academy of Sciences; Leibniz-Gemeinschaft; Science Mission Directorate; Agence Nationale de la Recherche; Max-Planck-Institut für Astronomie; European Commission; University of Oxford; Universidad Nacional Autónoma de México; Istituto Nazionale di Astrofisica; Durham University; University of Notre Dame; Carnegie Mellon University; University of Washington; Smithsonian Astrophysical Observatory; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Planetary Science Division; Carnegie Institution of Washington; University of Portsmouth; New Mexico State University; University of Utah; Ohio State University; Yale University; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; Macquarie University; W. M. Keck Foundation; Queen's University Belfast; Gordon and Betty Moore Foundation; Space Telescope Science Institute; Australian National University; Vanderbilt University; Javna Agencija za Raziskovalno Dejavnost RS; National Science Foundation","keywords":"Metallicity; Physics; Photometry (optics); Astrophysics; White dwarf; Stars; Binary number; Effective temperature; Astronomy; Mathematics","score_opus":0.00676302317147722,"score_gpt":0.20104246612915538,"score_spread":0.19427944295767816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221151631","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9522163,0.0004426901,0.042925783,0.000045561734,0.000023142118,0.000016952721,0.000877187,0.0005231643,0.0029291706],"genre_scores_gemma":[0.9824346,0.00009042724,0.016483227,0.000014879393,0.000013586126,0.000008911197,0.00053945644,0.000038465092,0.00037643645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989598,0.00025683298,0.00008908007,0.00037142285,0.00025285746,0.00007007817],"domain_scores_gemma":[0.9959138,0.0013067275,0.001024174,0.0008842676,0.00072015746,0.0001508572],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025890984,0.00058340916,0.00048787688,0.0016605147,0.0002994781,0.001505641,0.0004388805,0.0002726946,0.0007245229],"category_scores_gemma":[0.0063949763,0.00030856187,0.0002851227,0.0013975732,0.00030603382,0.0009098506,0.0009654794,0.00029072352,0.00053432095],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034313102,0.000047733523,0.8603876,0.00008434982,0.00017949415,0.00004718308,0.00027681096,0.022108188,0.03554247,0.0014043925,0.00045747004,0.07912114],"study_design_scores_gemma":[0.000032755594,0.00019526263,0.8379582,0.00006319656,0.00020749355,0.00024277315,0.00023127477,0.099963024,0.05158177,0.0023199725,0.0071508577,0.000053400112],"about_ca_topic_score_codex":0.003009917,"about_ca_topic_score_gemma":0.006690566,"teacher_disagreement_score":0.003009917,"about_ca_system_score_codex":0.00041923448,"about_ca_system_score_gemma":0.00033727082,"threshold_uncertainty_score":0.013692617},"labels":[],"label_agreement":null},{"id":"W4221152292","doi":"10.3847/1538-4357/ac5682","title":"Investigating the Low-flux States in Six Intermediate Polars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Flux (metallurgy); Accretion (finance); Astrophysics; Accretion disc; Photometry (optics); Intermediate polar; Materials science; Stars; White dwarf","score_opus":0.011463380379072057,"score_gpt":0.2307624513175423,"score_spread":0.21929907093847026,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221152292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99844474,0.0000457201,0.00019821968,0.0000111663985,0.0000032483679,0.0000034976092,0.000070150534,0.000007703364,0.001215581],"genre_scores_gemma":[0.9994535,0.000015983278,0.00011303105,0.000011937621,0.000003777963,0.0000027338765,0.00019031028,0.0000047864532,0.00020399115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993026,0.000006111817,0.0000036712597,0.000019256142,0.000011564945,0.000029158517],"domain_scores_gemma":[0.9996625,0.00005546502,0.00008647034,0.000023545874,0.00005283185,0.00011917519],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014199507,0.00020250521,0.00028786503,0.0010847294,0.00054878514,0.00093021546,0.00020137535,0.00027921973,0.0018628556],"category_scores_gemma":[0.00030520806,0.00015471055,0.00015594384,0.0004961719,0.0004068532,0.00021212267,0.00056299986,0.00037285106,0.00032839668],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010633639,0.00015048734,0.72068757,0.00005986286,0.00006740558,0.0008973173,0.0011900448,0.0005147847,0.2616646,0.00085899833,0.00040243127,0.012443103],"study_design_scores_gemma":[0.000011390427,0.00008441143,0.9912144,0.0000072744897,0.000015485322,0.00024109038,0.0004903547,0.0007475826,0.006273315,0.00016971273,0.0007358359,0.00000917566],"about_ca_topic_score_codex":0.0023503555,"about_ca_topic_score_gemma":0.003490627,"teacher_disagreement_score":0.0023503555,"about_ca_system_score_codex":0.00031982685,"about_ca_system_score_gemma":0.00008953826,"threshold_uncertainty_score":0.0062318444},"labels":[],"label_agreement":null},{"id":"W4221152614","doi":"10.3847/1538-4357/ac52f3","title":"Kinematics and Feedback in H ii Regions in the Dwarf Starburst Galaxy IC 10","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Star formation; Velocity dispersion; Luminosity; RADIUS; Irregular galaxy; Lenticular galaxy","score_opus":0.014110230705272557,"score_gpt":0.23904139979155695,"score_spread":0.22493116908628438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221152614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993038,0.000055449716,0.00005312639,0.0000054826373,7.9808075e-7,0.0000018272503,0.0001474806,0.000008389959,0.0004236306],"genre_scores_gemma":[0.9993625,0.000050288345,0.000118124146,0.000006070935,0.000001585336,0.0000015493622,0.00029181075,0.0000024320764,0.0001657294],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992967,0.00000433452,0.0000035352361,0.000022844377,0.000013785524,0.000025745245],"domain_scores_gemma":[0.9997489,0.000020227928,0.00009791242,0.0000119498645,0.000024924282,0.000096043164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008610093,0.00021512144,0.00016594034,0.00086544733,0.00022598339,0.00043594293,0.00019898382,0.00013683214,0.00080440316],"category_scores_gemma":[0.00025882685,0.00017674985,0.000115232084,0.00058161333,0.00021365884,0.00017889742,0.0003812305,0.00012560409,0.00016568768],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000761914,0.00002657849,0.9785065,0.000014237013,0.000031118743,0.00014049283,0.00026283012,0.00051650405,0.015953211,0.00006698005,0.00017021553,0.0042351405],"study_design_scores_gemma":[0.0000011475211,0.00001448379,0.99898344,0.0000021962744,0.0000057872735,0.00006405094,0.00009473449,0.00025651985,0.00039188276,0.000015896063,0.0001678798,0.0000019769795],"about_ca_topic_score_codex":0.030047182,"about_ca_topic_score_gemma":0.03870693,"teacher_disagreement_score":0.030047182,"about_ca_system_score_codex":0.00043751913,"about_ca_system_score_gemma":0.00015615989,"threshold_uncertainty_score":0.059744596},"labels":[],"label_agreement":null},{"id":"W4221154795","doi":"10.3847/1538-4357/ac6e65","title":"Milky Way Satellite Census. IV. Constraints on Decaying Dark Matter from Observations of Milky Way Satellite Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"SLAC National Accelerator Laboratory; Integrated Electronics Engineering Center, Binghamton University; European Regional Development Fund; Science and Technology Facilities Council; University of Illinois at Urbana-Champaign; Institut de Física d'Altes Energies; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Stanford Research Computing Center, Stanford University; European Commission; Ministerio de Ciencia e Innovación; Generalitat de Catalunya; Office of Science; University of Edinburgh; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; University of Sussex; University of Nottingham; National Aeronautics and Space Administration; University College London; Space Telescope Science Institute; University of Portsmouth; University of Chicago; Ohio State University; Ministério da Ciência, Tecnologia e Inovação; University of Michigan; High Energy Physics; Deutsche Forschungsgemeinschaft; Argonne National Laboratory; Centres de Recerca de Catalunya; U.S. Department of Energy; University of Cambridge; Fermilab; National Science Foundation","keywords":"Milky Way; Satellite galaxy; Satellite; Dwarf galaxy problem; Dark matter; Galaxy; Astronomy; Physics; Astrophysics; Geography; Galaxy formation and evolution; Galaxy group","score_opus":0.019324255503178588,"score_gpt":0.22915779407494372,"score_spread":0.20983353857176512,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221154795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99668413,0.00007524269,0.00035929127,0.00007691918,0.0000024917347,0.0000054127995,0.0020913917,0.000038237325,0.0006669554],"genre_scores_gemma":[0.99498415,0.000060201557,0.0005769401,0.000031423606,0.0000047216818,0.000011967697,0.004047388,0.00002968048,0.00025349428],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998235,0.000043041993,0.00001218809,0.000051429008,0.000035334808,0.000034611145],"domain_scores_gemma":[0.9989458,0.00028827952,0.00031746575,0.0001580909,0.000156139,0.00013430852],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008203224,0.0002958107,0.0003850574,0.00046365446,0.00029542766,0.0006659355,0.00084134657,0.00049680844,0.00088128116],"category_scores_gemma":[0.003821558,0.00032260746,0.00077422336,0.00061799143,0.00030030956,0.0007364872,0.00064475206,0.00033194854,0.00029046918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017200701,0.000047089306,0.7403027,0.00006708492,0.00022864832,0.00023048471,0.0002990321,0.2475799,0.002291903,0.0018099702,0.001786161,0.0051851124],"study_design_scores_gemma":[0.0001420144,0.00008797698,0.503331,0.00003951488,0.00008658198,0.000091283415,0.00022262763,0.48723048,0.002394402,0.0013187389,0.0050155967,0.00003978392],"about_ca_topic_score_codex":0.07954231,"about_ca_topic_score_gemma":0.05781647,"teacher_disagreement_score":0.07954231,"about_ca_system_score_codex":0.0012152212,"about_ca_system_score_gemma":0.0008155766,"threshold_uncertainty_score":0.15815866},"labels":[],"label_agreement":null},{"id":"W4221155515","doi":"10.3847/1538-4357/ac58f9","title":"Multiphase ISM in the z = 5.7 Hyperluminous Starburst SPT 0346–52","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"National Astronomical Observatory of Japan; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Max-Planck-Gesellschaft; National Institutes of Natural Sciences; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Space Telescope Science Institute; Alfred P. Sloan Foundation; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Interstellar medium; Metallicity; Star formation; Astronomy; Photoionization; Ionization","score_opus":0.0126305104818525,"score_gpt":0.24035130359998963,"score_spread":0.22772079311813714,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221155515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993393,0.000038091945,0.00015566619,0.000019697341,0.0000016638973,0.000001925562,0.00011819161,0.000021378408,0.00030405237],"genre_scores_gemma":[0.99963605,0.000017099388,0.00011031812,0.000007847829,0.0000015199527,0.0000011578707,0.00016021293,0.0000039531346,0.000061890234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999466,0.000005826662,0.0000040774994,0.000018604962,0.000008996068,0.00001593739],"domain_scores_gemma":[0.99981505,0.000024010433,0.00006611783,0.000013851215,0.000013781459,0.00006713752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010156105,0.00029923694,0.00023162964,0.00034443196,0.00034567527,0.0006409501,0.0004024131,0.0004417883,0.0011713783],"category_scores_gemma":[0.00029596756,0.00024304044,0.0003462985,0.0003068934,0.00028664494,0.0002789656,0.0003974271,0.00025838256,0.00022765552],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002710377,0.000113202106,0.94649434,0.000033967273,0.000092059614,0.0012990524,0.00022728612,0.018792842,0.027185038,0.0005153779,0.0004296178,0.0045461734],"study_design_scores_gemma":[0.0000689981,0.00012741747,0.9429917,0.000010742502,0.000041070518,0.0006173008,0.00024416874,0.05301579,0.0018431017,0.00039003414,0.00063790695,0.00001170348],"about_ca_topic_score_codex":0.012569712,"about_ca_topic_score_gemma":0.011594444,"teacher_disagreement_score":0.012569712,"about_ca_system_score_codex":0.00046644552,"about_ca_system_score_gemma":0.00015991133,"threshold_uncertainty_score":0.024993122},"labels":[],"label_agreement":null},{"id":"W4221155639","doi":"10.3847/1538-4357/ac6104","title":"Multiwavelength Variability of Sagittarius A* in 2019 July","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Institutes of Natural Sciences; Canada Research Chairs; Associated Universities; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Flare; Telescope; Flux (metallurgy); Astronomy; Materials science","score_opus":0.009621277384692052,"score_gpt":0.22536388903181176,"score_spread":0.21574261164711972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221155639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943738,0.000092298935,0.00022031959,0.000075132164,0.000015183881,0.000007842319,0.0022372406,0.000083176565,0.0028950784],"genre_scores_gemma":[0.9911726,0.000051211788,0.00034923822,0.000049219845,0.000019915842,0.000013388192,0.0071475264,0.000026796886,0.0011701648],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985003,0.000010613378,0.000010125193,0.000049991228,0.00004510985,0.000034107707],"domain_scores_gemma":[0.9995821,0.000020108086,0.00014434737,0.000038947204,0.000109876026,0.0001046734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019964935,0.00021600543,0.00019362739,0.001261843,0.0003433306,0.00070231734,0.00024491487,0.00021321786,0.0012485671],"category_scores_gemma":[0.00040346634,0.000101505575,0.00022631718,0.0008470878,0.00016789733,0.00022509742,0.0005433003,0.00018926771,0.00056986825],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031373688,0.000084882784,0.9568893,0.000028905979,0.0001674887,0.0002814874,0.00037861796,0.0006884514,0.022742046,0.00024171747,0.0024642665,0.015719095],"study_design_scores_gemma":[0.0000020024024,0.000034320015,0.99628335,0.0000026856683,0.000007931234,0.00005575105,0.00007049999,0.00020903762,0.00052455714,0.00002897102,0.0027773986,0.0000035293858],"about_ca_topic_score_codex":0.02181763,"about_ca_topic_score_gemma":0.038261365,"teacher_disagreement_score":0.02181763,"about_ca_system_score_codex":0.00075237494,"about_ca_system_score_gemma":0.0002461033,"threshold_uncertainty_score":0.043381274},"labels":[],"label_agreement":null},{"id":"W4221157511","doi":"10.3847/1538-4357/ac609d","title":"On the Spectral Evolution of Hot White Dwarf Stars. III. The PG 1159–DO–DB–DQ Evolutionary Channel Revisited","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"White dwarf; Physics; Astrophysics; Stars; Stellar classification; Astronomy","score_opus":0.009870590328103083,"score_gpt":0.2083303320639422,"score_spread":0.1984597417358391,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221157511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9880903,0.00015177677,0.0068748146,0.00015994417,0.000008610351,0.0000118859,0.00015601247,0.00010398598,0.004442669],"genre_scores_gemma":[0.9990445,0.00005000872,0.0004769304,0.000019981668,0.0000040231657,0.000004188181,0.000048075213,0.000020010557,0.00033222776],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999397,0.000018571398,0.0000026138855,0.0000118388825,0.000010867181,0.000016445112],"domain_scores_gemma":[0.9997503,0.00011541651,0.000044875713,0.000033135064,0.000023483153,0.00003276046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036715806,0.0003482145,0.00034487128,0.0004024442,0.00036581504,0.0005441834,0.00048233013,0.0004897341,0.0014849643],"category_scores_gemma":[0.0010262746,0.00015101256,0.00041836555,0.00024926127,0.0005478575,0.00046974988,0.0005078459,0.00026870766,0.00019032473],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022580307,0.00007069522,0.0939769,0.000094455696,0.00008144189,0.0005317662,0.00021166283,0.8626017,0.015135224,0.01781286,0.0004888511,0.008768703],"study_design_scores_gemma":[0.000053529013,0.000060092756,0.030298539,0.000013667072,0.000025129348,0.00007230122,0.00009101703,0.96114826,0.0032077143,0.004217848,0.00079749903,0.000014248541],"about_ca_topic_score_codex":0.007894964,"about_ca_topic_score_gemma":0.0033642838,"teacher_disagreement_score":0.007894964,"about_ca_system_score_codex":0.0006393913,"about_ca_system_score_gemma":0.00023593214,"threshold_uncertainty_score":0.015698016},"labels":[],"label_agreement":null},{"id":"W4221158297","doi":"10.3847/1538-4357/aca1c3","title":"Pegasus IV: Discovery and Spectroscopic Confirmation of an Ultra-faint Dwarf Galaxy in the Constellation Pegasus","year":2023,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; Office of Science; National Centre for Supercomputing Applications; Eidgenössische Technische Hochschule Zürich; Institut de Física d'Altes Energies; University of Sussex; Center for Cosmology and Astroparticle Physics, Ohio State University; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; High Energy Physics; Deutsche Forschungsgemeinschaft; University of Illinois at Urbana-Champaign; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Agencia Nacional de Investigación y Desarrollo; University of Portsmouth; University of Chicago; Kavli Institute for Cosmological Physics, University of Chicago; University of California, Santa Cruz; Ohio State University; University College London; National Aeronautics and Space Administration; U.S. Department of Energy; European Space Agency; Fermilab; Laboratory Directed Research and Development; National Science Foundation","keywords":"Physics; Constellation; Astronomy; Astrophysics; Galaxy; Dwarf galaxy","score_opus":0.014226834014573484,"score_gpt":0.24423244040291323,"score_spread":0.23000560638833975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221158297","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98890465,0.0005158291,0.0015508627,0.0004071324,0.00007194927,0.000032600532,0.00089317927,0.00019405916,0.00742975],"genre_scores_gemma":[0.9962469,0.00009015681,0.0013968116,0.00008657985,0.00004347716,0.000008537011,0.00077732746,0.000027201915,0.0013229912],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999813,0.000017462098,0.000009198133,0.00007463826,0.000046316287,0.000039314156],"domain_scores_gemma":[0.99961394,0.00002376216,0.000112662165,0.00008668651,0.000038958624,0.00012408616],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002605757,0.0003498838,0.00027417875,0.0009503192,0.0007737115,0.0007911164,0.000541303,0.00053561816,0.001501624],"category_scores_gemma":[0.0006986258,0.00018564657,0.00023969097,0.0003863515,0.0006844564,0.00036921634,0.0013157768,0.0005456848,0.0008929065],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011625021,0.00022790846,0.73410845,0.00018345489,0.0002179815,0.010392912,0.0025571329,0.0008398228,0.15096894,0.0053505423,0.009817367,0.084173],"study_design_scores_gemma":[0.000069087495,0.00046438762,0.8727044,0.00006044411,0.0001137369,0.009516906,0.00085422996,0.0017832229,0.020586247,0.0033024696,0.09049913,0.000045833112],"about_ca_topic_score_codex":0.0040091374,"about_ca_topic_score_gemma":0.002188108,"teacher_disagreement_score":0.0040091374,"about_ca_system_score_codex":0.00065782416,"about_ca_system_score_gemma":0.00022957982,"threshold_uncertainty_score":0.007971585},"labels":[],"label_agreement":null},{"id":"W4221158541","doi":"10.3847/1538-4357/ac5d55","title":"Photometric Signature of Ultraharmonic Resonances in Barred Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Smithsonian Astrophysical Observatory; Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Carnegie Institution for Science; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Barred spiral galaxy; Bar (unit); Astrophysics; Galaxy rotation curve; Galaxy; Lenticular galaxy; Galaxy formation and evolution","score_opus":0.00986316019404203,"score_gpt":0.22165703279289706,"score_spread":0.21179387259885502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221158541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918956,0.000013381441,0.00038064108,0.0000050880108,9.452405e-7,0.0000013277198,0.000025072502,0.000018486935,0.00036558046],"genre_scores_gemma":[0.99980813,0.0000022128988,0.00012305286,0.0000018430769,6.9463755e-7,4.5730775e-7,0.000028353106,0.000001959163,0.00003334176],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999198,0.000012671843,0.000003206215,0.000027623715,0.000019130957,0.000017602328],"domain_scores_gemma":[0.9995629,0.00008533242,0.00014841816,0.00006109925,0.00004957348,0.00009254393],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023222937,0.000092356466,0.00015375845,0.00067396276,0.00018440561,0.00036483954,0.00025614438,0.00018277047,0.00093675574],"category_scores_gemma":[0.000727775,0.00013835194,0.000120421595,0.00022600924,0.00032847933,0.00016382296,0.00039357238,0.00017703051,0.0001520036],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034035547,0.0000934472,0.92182183,0.000021088827,0.000062661784,0.00028512414,0.00073590013,0.0064538796,0.05911303,0.0011606375,0.00023417152,0.0096778795],"study_design_scores_gemma":[0.000010153336,0.000050242503,0.9789634,0.0000036253034,0.000010317291,0.00008657655,0.000108896726,0.018121228,0.0021580812,0.00022020812,0.00026069037,0.0000065016866],"about_ca_topic_score_codex":0.0020147313,"about_ca_topic_score_gemma":0.0020970101,"teacher_disagreement_score":0.0020147313,"about_ca_system_score_codex":0.00025054815,"about_ca_system_score_gemma":0.0000488114,"threshold_uncertainty_score":0.004006088},"labels":[],"label_agreement":null},{"id":"W4221160004","doi":"10.3847/1538-4357/ac8c26","title":"Radio Analysis of SN2004C Reveals an Unusual CSM Density Profile as a Harbinger of Core Collapse","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Heising-Simons Foundation; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Supernova; RADIUS; Stars; Context (archaeology); Spectral energy distribution; Galaxy","score_opus":0.015898991319149153,"score_gpt":0.2558740944656672,"score_spread":0.23997510314651807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221160004","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998869,0.000028305114,0.00023538731,0.0000073843935,0.0000010469133,0.0000027082629,0.00020475764,0.000018928977,0.00063249917],"genre_scores_gemma":[0.99872726,0.000015243756,0.00023590242,0.000008398932,0.0000021294902,0.000002991737,0.000686397,0.000004995107,0.0003166112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999509,0.0000044873223,0.000002428387,0.000011459348,0.000016140417,0.000014739064],"domain_scores_gemma":[0.9998357,0.000015313362,0.000045739762,0.000018353916,0.00003635958,0.000048485792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015213019,0.00015190072,0.000115914925,0.0011451937,0.00024582024,0.0003133218,0.000179015,0.00015387298,0.0008187633],"category_scores_gemma":[0.00028138838,0.00010307479,0.00015441196,0.00041004896,0.00013658588,0.00008100865,0.00020766932,0.00015510611,0.00019533095],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037435448,0.00008560985,0.78429025,0.000015426247,0.00004367268,0.0011482239,0.00018899633,0.0009245361,0.20294447,0.0003386652,0.00053322036,0.0091125555],"study_design_scores_gemma":[0.0000022757097,0.00003864088,0.9952761,0.0000014538645,0.0000051772367,0.00030514546,0.000043760847,0.0012933394,0.0026318082,0.000037747028,0.00036142458,0.0000031615355],"about_ca_topic_score_codex":0.008655381,"about_ca_topic_score_gemma":0.010071348,"teacher_disagreement_score":0.008655381,"about_ca_system_score_codex":0.000347196,"about_ca_system_score_gemma":0.00009378462,"threshold_uncertainty_score":0.017210007},"labels":[],"label_agreement":null},{"id":"W4221161472","doi":"10.3847/1538-4357/ac5f04","title":"Science-driven Tunable Design of Cosmic Explorer Detectors","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":107,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Science Foundation","keywords":"Physics; Gravitational wave; Detector; Neutron star; Sensitivity (control systems); COSMIC cancer database; LIGO; Binary number; Astrophysics; Astronomy; Optics; Electronic engineering","score_opus":0.02581470826626431,"score_gpt":0.306655362585565,"score_spread":0.28084065431930066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221161472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.79199094,0.00087166816,0.17448151,0.00089106185,0.00017072627,0.0005204005,0.00085355894,0.0042055333,0.026014535],"genre_scores_gemma":[0.97067845,0.000055989687,0.027313631,0.00019752004,0.000015605992,0.0001291458,0.00017102658,0.00011309883,0.0013255256],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99885595,0.00018793833,0.000054744316,0.00033994453,0.00030826134,0.00025316243],"domain_scores_gemma":[0.9985043,0.00036066573,0.00034577362,0.00018698185,0.00042168165,0.0001806406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013564606,0.0007647845,0.00049564673,0.0008721254,0.00038099033,0.0013532566,0.0025087867,0.0011307709,0.0034563865],"category_scores_gemma":[0.002607268,0.00042133528,0.0003109975,0.0003666628,0.0005034754,0.0010230722,0.0011740995,0.0004749509,0.0011015659],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0029068235,0.0004672557,0.03367969,0.00045850012,0.000374749,0.0005117993,0.00028111416,0.105358936,0.7561153,0.021472046,0.0063182963,0.072055526],"study_design_scores_gemma":[0.00052356167,0.0015730803,0.011167621,0.000062473184,0.00016993993,0.0006943331,0.00011610932,0.31774595,0.63162786,0.0055569094,0.030568074,0.00019411727],"about_ca_topic_score_codex":0.0007505092,"about_ca_topic_score_gemma":0.000878712,"teacher_disagreement_score":0.0034563865,"about_ca_system_score_codex":0.0014651618,"about_ca_system_score_gemma":0.0006685405,"threshold_uncertainty_score":0.011562765},"labels":[],"label_agreement":null},{"id":"W4221161529","doi":"10.3847/1538-4357/acd770","title":"Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO–Virgo Observing Run O3a","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; University of Waterloo; University of Toronto; Université de Montréal; Canadian Institute for Theoretical Astrophysics; Polytechnique Montréal; McGill University; University of British Columbia","funders":"National Research, Development and Innovation Office; Institute for Cosmic Ray Research, University of Tokyo; Science and Engineering Research Board; Japan Society for the Promotion of Science; Australian Research Council; McGill Space Institute; Smithsonian Astrophysical Observatory; Great Southern Development Commission, Government of Western Australia; Agencia Estatal de Investigación; Govern de les Illes Balears; Institut Périmètre de physique théorique; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; Ministry of Education, India; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Hungarian Scientific Research Fund; University of Toronto; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; McGill University; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; National Research Council Canada; Fundacja na rzecz Nauki Polskiej; U.S. Department of Energy; Agence Nationale de la Recherche; Kavli Foundation; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Korea Institute of Science and Technology Information; Fondation familiale Trottier; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Culture, Sports, Science and Technology; European Regional Development Fund; ICTP South American Institute for Fundamental Research; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; Russian Science Foundation; University of British Columbia; Scottish Funding Council; National Astronomical Observatory of Japan; Canadian Institute for Advanced Research; Centres de Recerca de Catalunya; Institut des Origines de Lyon; Abdus Salam International Centre for Theoretical Physics; Government of Canada; Industry Canada; Associated Universities; Academia Sinica; Ministerio de Ciencia e Innovación; European Social Fund; Royal Society; National Science Foundation","keywords":"LIGO; Physics; Gravitational wave; Astronomy; Astrophysics","score_opus":0.013709169905118555,"score_gpt":0.28855444871666147,"score_spread":0.2748452788115429,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221161529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99710804,0.00007098944,0.00042924212,0.00005298267,0.0000020332038,0.000009431207,0.0009929085,0.00007855522,0.0012558933],"genre_scores_gemma":[0.9970795,0.00002643363,0.00049118674,0.000021971944,0.000004195291,0.000004357477,0.002121076,0.000012494821,0.00023888894],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996649,0.000040151608,0.000009216419,0.000072490264,0.00012311022,0.00009013089],"domain_scores_gemma":[0.9988582,0.00022726478,0.0004051023,0.00010145858,0.00010334439,0.0003046422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069069385,0.0002709895,0.00027087942,0.0013256612,0.00065794424,0.00066996925,0.00034399275,0.00033756578,0.0014079161],"category_scores_gemma":[0.0012006075,0.00016730573,0.000446879,0.0009801745,0.00031403263,0.00020723516,0.00057935435,0.00025966478,0.0002449079],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002667397,0.000037281814,0.9814249,0.000020069285,0.00013346369,0.00016118519,0.00017794405,0.0014526001,0.009562931,0.00024360718,0.0006891656,0.0058299913],"study_design_scores_gemma":[0.00000969976,0.000038926428,0.9943399,0.000005626375,0.000029472452,0.000063439045,0.00008760919,0.0033462502,0.001276058,0.00005710546,0.00073703023,0.000008944944],"about_ca_topic_score_codex":0.09176899,"about_ca_topic_score_gemma":0.16728112,"teacher_disagreement_score":0.09176899,"about_ca_system_score_codex":0.0010810395,"about_ca_system_score_gemma":0.000601669,"threshold_uncertainty_score":0.18246967},"labels":[],"label_agreement":null},{"id":"W4221161571","doi":"10.3847/1538-4357/ac6def","title":"Search for Spatial Correlations of Neutrinos with Ultra-high-energy Cosmic Rays","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Institute for Global Prominent Research, Chiba University; Institute for Cosmic Ray Research, University of Tokyo; Institut National de Physique Nucléaire et de Physique des Particules; Agencia Nacional de Promoción Científica y Tecnológica; Fundação para a Ciência e a Tecnologia; Deutsches Elektronen-Synchrotron; U.S. Bureau of Land Management; U.S. Air Force; Office of Science; Conseil Régional d'Alsace; Istituto Nazionale di Fisica Nucleare; Marsden Fund; Helmholtz Alliance for Astroparticle Physics; Ministry of Science and Higher Education of the Russian Federation; RIKEN; Junta de Andalucía; Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España; Conseil Régional Provence-Alpes-Côte d'Azur; Chiba University; RWTH Aachen University; Vetenskapsrådet; Unitatea Executiva pentru Finantarea Invatamantului Superior, a Cercetarii, Dezvoltarii si Inovarii; Financiadora de Estudos e Projetos; Japan Society for the Promotion of Science; Villum Fonden; Institut Universitaire de France; Centre National de la Recherche Scientifique; College of Engineering, Michigan State University; Knut och Alice Wallenbergs Stiftelse; Conseil Régional, Île-de-France; Fonds De La Recherche Scientifique - FNRS; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Labex UnivEarthS; Ministero dell’Istruzione, dell’Università e della Ricerca; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Generalitat Valenciana; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Consejo Nacional de Ciencia y Tecnología; Fonds Wetenschappelijk Onderzoek; Universidad Nacional Autónoma de México; Istituto Nazionale di Astrofisica; Consejo Nacional de Investigaciones Científicas y Técnicas; Natural Sciences and Engineering Research Council of Canada; Bundesministerium für Bildung und Forschung; Vlaamse regering; National Research Foundation; Javna Agencija za Raziskovalno Dejavnost RS; Xunta de Galicia; Strong; Colegiul Consultativ pentru Cercetare-Dezvoltare şi Inovare; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Grainger Foundation; Agence Nationale de la Recherche; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; University of Oxford; Ministerul Cercetării, Inovării şi Digitalizării; Western Canada Research Grid; European Commission; Fundação de Amparo à Pesquisa do Estado de São Paulo; “la Caixa” Foundation; University of Utah; Arab Fund for Economic and Social Development; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Marquette University; Ministerio de Ciencia, Innovación y Universidades; Polarforskningssekretariatet; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; U.S. Department of Energy; University of Wisconsin-Madison; National Research Foundation of Korea; University of Tokyo; Fermilab; Office of Polar Programs; Michigan State University; Compute Canada; Belgian Federal Science Policy Office; National Science Foundation","keywords":"Physics; Neutrino; Pierre Auger Observatory; Cosmic neutrino background; Cosmic ray; Astrophysics; Neutrino detector; Astronomy; Solar neutrino problem; Astroparticle physics; Solar neutrino; Neutrino oscillation; Particle physics","score_opus":0.008901674479510503,"score_gpt":0.21456879500617426,"score_spread":0.20566712052666375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221161571","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99442405,0.00012853983,0.004561873,0.000036769972,0.0000058492255,0.0000055752203,0.00025390525,0.0000556244,0.0005279031],"genre_scores_gemma":[0.99771047,0.000028458911,0.0016562437,0.000014871362,0.0000112560665,0.0000028267038,0.00045726425,0.000013047183,0.00010554536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991762,0.00025355633,0.000036486435,0.0002712946,0.00016641163,0.00009612208],"domain_scores_gemma":[0.9954632,0.0016258865,0.0015372261,0.0005689907,0.0004134726,0.00039129812],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001392931,0.00036754855,0.00041365056,0.002124847,0.0005495929,0.0010566878,0.000465815,0.0004268861,0.0017674193],"category_scores_gemma":[0.0029185656,0.00025809498,0.00067702745,0.0018101119,0.0005715153,0.00039401892,0.0008246967,0.00040821914,0.00027115332],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024583336,0.000039177823,0.97667605,0.000016977925,0.00032897017,0.00014947579,0.000061151346,0.001783476,0.014636774,0.00085581135,0.00018342142,0.005022937],"study_design_scores_gemma":[0.000026369245,0.00010290781,0.9732197,0.000012425576,0.00017820905,0.00035936033,0.00022953615,0.015797252,0.007818644,0.0012620362,0.00097124506,0.000022213899],"about_ca_topic_score_codex":0.0023917116,"about_ca_topic_score_gemma":0.0029794148,"teacher_disagreement_score":0.0023917116,"about_ca_system_score_codex":0.0002671497,"about_ca_system_score_gemma":0.00032924218,"threshold_uncertainty_score":0.0073665977},"labels":[],"label_agreement":null},{"id":"W4221164245","doi":"10.3847/1538-4357/ac63ab","title":"The Appearance of Vortices in Protoplanetary Disks in Near-infrared Scattered Light","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Simon Fraser University","funders":"Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation","keywords":"Physics; Vortex; Protoplanetary disk; Astrophysics; Radiative transfer; Instability; Planet; Planetesimal; Astronomy; Optics; Mechanics","score_opus":0.0073621657216316385,"score_gpt":0.22573057759675277,"score_spread":0.21836841187512113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221164245","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991585,0.00001648744,0.00043449644,0.000007772156,0.0000013933739,0.0000021110081,0.00002015296,0.000014470367,0.00034454186],"genre_scores_gemma":[0.9995222,0.000007865674,0.0003316606,0.0000036229833,0.0000010976837,0.0000013282759,0.00004059335,0.000003591133,0.00008810183],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999764,0.0000032601342,8.9099575e-7,0.000004801492,0.0000071492445,0.0000075562143],"domain_scores_gemma":[0.9998628,0.000024434292,0.00002835901,0.000012859695,0.000029748173,0.000041776937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006722501,0.000113882794,0.0000923356,0.00042497512,0.00022008157,0.00038854268,0.00012730849,0.00016287084,0.0006062233],"category_scores_gemma":[0.00018758213,0.00012300971,0.00015462235,0.0001412231,0.00023173547,0.00016279833,0.00017984699,0.0001741178,0.00008848904],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065483374,0.00030940477,0.26321375,0.00006435221,0.00009360075,0.0010397169,0.000587207,0.031272963,0.6851859,0.002207063,0.0005087104,0.014862463],"study_design_scores_gemma":[0.00010620137,0.00041024736,0.65765095,0.000026948268,0.000043988843,0.0006170333,0.0008290074,0.25138974,0.08610048,0.0015412186,0.0012408292,0.000043399967],"about_ca_topic_score_codex":0.0010240142,"about_ca_topic_score_gemma":0.0008822074,"teacher_disagreement_score":0.0010240142,"about_ca_system_score_codex":0.0002447753,"about_ca_system_score_gemma":0.00007046717,"threshold_uncertainty_score":0.0020360947},"labels":[],"label_agreement":null},{"id":"W4221164445","doi":"10.3847/1538-4357/ac5c58","title":"The Double Detonation of a Double-degenerate System, from Type Ia Supernova Explosion to its Supernova Remnant","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Division of Mathematical Sciences; National Astronomical Observatory of Japan; Natural Sciences and Engineering Research Council of Canada; RIKEN; Japan Society for the Promotion of Science; Canadian Space Agency","keywords":"Ejecta; Supernova; Physics; Astrophysics; White dwarf; Detonation; Degenerate energy levels; Light curve; Deflagration; Thermonuclear fusion; Astronomy; Explosive material; Stars; Plasma; Chemistry; Nuclear physics","score_opus":0.02351419238900801,"score_gpt":0.25284881158516687,"score_spread":0.22933461919615886,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221164445","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944043,0.00029233767,0.0029744187,0.000017686398,0.000020765076,0.000009149734,0.0001149207,0.000086987035,0.0020794405],"genre_scores_gemma":[0.99822706,0.00008820132,0.00089554535,0.000010502948,0.0000071239806,0.0000023710427,0.00016103798,0.000008345235,0.0005997409],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996364,0.000002568509,0.0000029858431,0.000013386139,0.0000097685925,0.000007651431],"domain_scores_gemma":[0.99991524,0.000006629345,0.000030174682,0.000013828197,0.000009074826,0.000025125672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000100393445,0.0002241792,0.000115053335,0.00032308485,0.00020646637,0.0005070345,0.00013384088,0.00019249014,0.00079276005],"category_scores_gemma":[0.0002577394,0.00014068159,0.00020540097,0.00017709097,0.0002031587,0.00020090223,0.00055934343,0.00023713507,0.00020934785],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00097184774,0.000119417666,0.2852422,0.00019894414,0.00015098427,0.011660132,0.00034257077,0.008636508,0.64224285,0.004195716,0.00091120665,0.04532767],"study_design_scores_gemma":[0.00004044041,0.00073540077,0.84423435,0.00003092293,0.000110824105,0.021707483,0.0003197265,0.027626386,0.09239651,0.0039379518,0.008815102,0.000044948378],"about_ca_topic_score_codex":0.000653321,"about_ca_topic_score_gemma":0.000610231,"teacher_disagreement_score":0.00079276005,"about_ca_system_score_codex":0.00014461382,"about_ca_system_score_gemma":0.00009153746,"threshold_uncertainty_score":0.0026521087},"labels":[],"label_agreement":null},{"id":"W4221164854","doi":"10.3847/1538-4357/ac6504","title":"The Large Dispersion and Scattering of FRB 20190520B Are Dominated by the Host Galaxy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Science Foundation","keywords":"Physics; Galaxy; Fast radio burst; Scattering; Astrophysics; Analytical Chemistry (journal); Optics; Chemistry","score_opus":0.005727507779743536,"score_gpt":0.270801493196972,"score_spread":0.2650739854172285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221164854","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952135,0.00013991298,0.00020804886,0.00006161988,0.0000053653916,0.0000032149906,0.0007026222,0.000044489385,0.0036212497],"genre_scores_gemma":[0.99784636,0.000027488466,0.0001349545,0.000041804127,0.000006025822,0.0000026259047,0.0014374763,0.000012692011,0.00049052003],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998683,0.0000061003284,0.000005566534,0.000040691488,0.000035028716,0.000044304947],"domain_scores_gemma":[0.9996214,0.000036840564,0.00014368417,0.00003819147,0.000057435504,0.00010240665],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016774196,0.00025998484,0.000252716,0.0008236879,0.000452618,0.00063749554,0.00022368855,0.00022636745,0.0032837365],"category_scores_gemma":[0.00037937824,0.00016447582,0.00018125869,0.0004432474,0.00017980037,0.00015146508,0.0003010632,0.00021477733,0.0010419893],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006214121,0.00008780259,0.7934726,0.0000460127,0.0001024527,0.00069261744,0.00038342038,0.001046828,0.17826943,0.0006539265,0.004065501,0.02055787],"study_design_scores_gemma":[0.0000063968128,0.00002624755,0.99662447,0.00000350348,0.000007520042,0.00011117256,0.000080160855,0.00054605736,0.0016152189,0.00006318651,0.00091213983,0.000004034073],"about_ca_topic_score_codex":0.019186907,"about_ca_topic_score_gemma":0.017703613,"teacher_disagreement_score":0.019186907,"about_ca_system_score_codex":0.0006839579,"about_ca_system_score_gemma":0.00009346428,"threshold_uncertainty_score":0.03815049},"labels":[],"label_agreement":null},{"id":"W4221165309","doi":"10.3847/1538-4357/ac551b","title":"The Role of Disk Tearing and Precession in the Observed Variability of Pleione","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Precession; Accretion disc; Radiative transfer; Phase (matter); Magnetohydrodynamic drive; Angular momentum; Magnetohydrodynamics; Dynamo","score_opus":0.011450600810859819,"score_gpt":0.22453629485470766,"score_spread":0.21308569404384783,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221165309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99820936,0.000108816224,0.0004027783,0.000052699485,0.0000043789078,0.0000028109594,0.000532642,0.00005817879,0.00062835007],"genre_scores_gemma":[0.99914646,0.000023460889,0.00015481576,0.000008954474,0.0000029279097,0.000001955683,0.00052764657,0.000015662295,0.000118038704],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989414,0.000018831399,0.000009333455,0.00004506063,0.00001334712,0.000019358444],"domain_scores_gemma":[0.9994006,0.00016498177,0.0001536726,0.00012701958,0.00005740311,0.000096216405],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033637043,0.00024153038,0.0001931487,0.00045706404,0.00034762739,0.0007945165,0.00034907152,0.000282026,0.0012515903],"category_scores_gemma":[0.0016189466,0.00027191264,0.00028617444,0.00033452502,0.0003529029,0.00051631243,0.0004990867,0.00036654747,0.00027769056],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026145836,0.00003168391,0.96449715,0.00005697787,0.00009441764,0.00031748443,0.00046405633,0.0050277165,0.022961214,0.00027165338,0.0005204363,0.005495735],"study_design_scores_gemma":[0.000008643084,0.000024041718,0.9934009,0.000009245707,0.00001632161,0.000105802836,0.00008518337,0.0046321857,0.0008345977,0.00010364526,0.0007704992,0.00000906994],"about_ca_topic_score_codex":0.006704978,"about_ca_topic_score_gemma":0.007799691,"teacher_disagreement_score":0.006704978,"about_ca_system_score_codex":0.00041786392,"about_ca_system_score_gemma":0.00016734355,"threshold_uncertainty_score":0.01333189},"labels":[],"label_agreement":null},{"id":"W4221165467","doi":"10.3847/1538-4357/ac743f","title":"The Time Domain Spectroscopic Survey: Changing-look Quasar Candidates from Multi-epoch Spectroscopy in SDSS-IV","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Bishop's University","funders":"Lawrence Berkeley National Laboratory; Planetary Science Division; Deutsches Elektronen-Synchrotron; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Max-Planck-Institut für Astrophysik; Eötvös Loránd Tudományegyetem; National Central University; Max-Planck-Gesellschaft; Ministério da Ciência, Tecnologia e Inovação; Queen's University; Queen's University Belfast; Weizmann Institute of Science; University of Oxford; Durham University; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Office of Science; Max-Planck-Institut für Astronomie; University of Edinburgh; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; Stockholms Universitet; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; National Science Foundation","keywords":"Quasar; Astrophysics; Physics; Supermassive black hole; Emission spectrum; Active galactic nucleus; Spectroscopy; Spectral line; Population; Astronomy; Galaxy; Demography","score_opus":0.007005675248269318,"score_gpt":0.22334181363520536,"score_spread":0.21633613838693605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221165467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992649,0.00003059513,0.00014892465,0.00001007286,0.0000011637342,0.000009160559,0.00037731425,0.000008134394,0.00014964418],"genre_scores_gemma":[0.9982711,0.000023402967,0.00035853576,0.000011733795,0.0000036762613,0.000006797959,0.0011857135,0.0000032703897,0.00013561989],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996742,0.000041392028,0.0000373103,0.00008313363,0.00009320474,0.000070817296],"domain_scores_gemma":[0.9975782,0.0003658967,0.00085784495,0.00025101792,0.00039751682,0.00054945285],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007106514,0.00020964787,0.00017751835,0.0029460115,0.0003459659,0.0005388111,0.00038147296,0.00023074969,0.0007702124],"category_scores_gemma":[0.0013640864,0.00011518682,0.0002159521,0.0013543345,0.00020654514,0.00030278772,0.00084628386,0.00020261433,0.00032348244],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003203641,0.000020967373,0.9943124,0.000005474932,0.000010347748,0.00010267325,0.000113628215,0.00006492532,0.0027822435,0.000020862339,0.00011255531,0.0024218007],"study_design_scores_gemma":[0.0000021365463,0.000024445533,0.99876803,0.0000018328258,0.0000054178304,0.00015038635,0.00013403257,0.0003103887,0.00036985104,0.000011311625,0.0002199219,0.0000021163585],"about_ca_topic_score_codex":0.0045659943,"about_ca_topic_score_gemma":0.009723933,"teacher_disagreement_score":0.0045659943,"about_ca_system_score_codex":0.00021631974,"about_ca_system_score_gemma":0.00017228318,"threshold_uncertainty_score":0.009078801},"labels":[],"label_agreement":null},{"id":"W4221166016","doi":"10.3847/1538-4357/ac47a1","title":"Toward RNA Life on Early Earth: From Atmospheric HCN to Biomolecule Production in Warm Little Ponds","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Origins and Evolution of Life","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Atmosphere (unit); Early Earth; Hydrogen cyanide; Meteorite; Astrobiology; Abiogenesis; Earth (classical element); Atmospheric chemistry; Chemistry; Environmental chemistry; Hydrogen; Photodissociation; Nucleobase; Atmospheric sciences; Earth science; Environmental science; Meteorology; Geology; Photochemistry; Inorganic chemistry; Physics; Organic chemistry; DNA","score_opus":0.013402626654729407,"score_gpt":0.2313005403982331,"score_spread":0.2178979137435037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221166016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9674414,0.00017599446,0.026620846,0.00028703836,0.000025314539,0.000023888733,0.00018965438,0.0001378104,0.0050979718],"genre_scores_gemma":[0.9950865,0.0001040254,0.0036227563,0.00004816702,0.000008169849,0.000020853247,0.000076352975,0.00003476544,0.0009982858],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999534,0.0000093158205,0.0000015701044,0.000010724305,0.000011217815,0.000013795202],"domain_scores_gemma":[0.9998381,0.000059472553,0.000030251935,0.000015861368,0.000019378878,0.0000367843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016442453,0.00027018637,0.00040387484,0.0002545728,0.0004739982,0.0006984716,0.00061157456,0.0008804431,0.0016404118],"category_scores_gemma":[0.00074250076,0.00033729928,0.0005773701,0.00024592222,0.0008078449,0.0007264332,0.00059884426,0.00068369065,0.00015699073],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037258895,0.000050585182,0.0071698716,0.00003635115,0.00002141597,0.00018921899,0.000065737484,0.9681281,0.015640842,0.007217909,0.00016867343,0.0012741527],"study_design_scores_gemma":[0.0000192909,0.000023095628,0.0021471097,0.0000040430446,0.000004723945,0.000020511823,0.000026334437,0.99233234,0.0019159443,0.0032461726,0.00025095025,0.000009437647],"about_ca_topic_score_codex":0.011552142,"about_ca_topic_score_gemma":0.004402148,"teacher_disagreement_score":0.011552142,"about_ca_system_score_codex":0.0012394907,"about_ca_system_score_gemma":0.00059252867,"threshold_uncertainty_score":0.022969842},"labels":[],"label_agreement":null},{"id":"W4221166769","doi":"10.3847/1538-4357/ac5c2c","title":"Understanding the Nature of an Unusual Post-starburst Quasar with Exceptionally Strong Ne v Emission","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Heising-Simons Foundation; Space Telescope Science Institute; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; University of Arizona; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Galaxy; Quasar; Star formation; Outflow; Population; Astronomy; Extinction (optical mineralogy); Emission spectrum; Spectral line","score_opus":0.014766573153232323,"score_gpt":0.2302295049623781,"score_spread":0.21546293180914577,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221166769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99888974,0.00017697678,0.00021836237,0.000056810295,0.0000023447851,0.0000017863039,0.00006811913,0.000007703263,0.00057810993],"genre_scores_gemma":[0.9995939,0.00006507998,0.00011640063,0.00001929256,0.000007215974,6.3605694e-7,0.00007181898,0.0000010773883,0.00012453986],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999622,0.0000026082769,0.0000023394048,0.000010366953,0.000007148277,0.000015323483],"domain_scores_gemma":[0.99981207,0.000016621027,0.000093030925,0.000010223524,0.000021381426,0.000046650715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012567824,0.00010282358,0.00010843467,0.00045946726,0.00019482631,0.0004782653,0.00019642127,0.00024604087,0.00080089335],"category_scores_gemma":[0.00020332751,0.00006634942,0.00007784935,0.00020157917,0.0002602656,0.0003103311,0.00019819837,0.00015879709,0.00014312593],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006684416,0.000042784173,0.9057913,0.000027421067,0.000018832623,0.0027657584,0.00025887488,0.00014335108,0.083515994,0.00034301993,0.00023151505,0.00679437],"study_design_scores_gemma":[0.0000014848816,0.00003197661,0.9948578,0.0000041094995,0.0000056850313,0.0022320421,0.00020610173,0.00026353475,0.0015717031,0.00014935093,0.0006732214,0.0000028967097],"about_ca_topic_score_codex":0.0011531936,"about_ca_topic_score_gemma":0.0020398155,"teacher_disagreement_score":0.0011531936,"about_ca_system_score_codex":0.00015112635,"about_ca_system_score_gemma":0.000051873307,"threshold_uncertainty_score":0.0026792884},"labels":[],"label_agreement":null},{"id":"W4221167645","doi":"10.3847/1538-4357/ac75f0","title":"Weak Mass Loss from the Red Supergiant Progenitor of the Type II SN 2021yja","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"College of Engineering, Michigan State University; Jet Propulsion Laboratory; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; NASA Exoplanet Science Institute; W. M. Keck Foundation; Space Telescope Science Institute; National Science Foundation; University of Washington; Science and Technology Facilities Council; Michigan State University; Agencia Nacional de Investigación y Desarrollo; Washington Research Foundation; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; University of North Carolina at Chapel Hill; California Institute of Technology","keywords":"Supernova; Red supergiant; Physics; Astrophysics; Supergiant; Light curve; Progenitor; Luminosity; Pair-instability supernova; Galaxy; Astronomy; Ejecta; Stars; Progenitor cell","score_opus":0.009369687448737526,"score_gpt":0.21293049759598168,"score_spread":0.20356081014724414,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4221167645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99911946,0.00008531164,0.00011903074,0.000008922572,0.000002289575,0.0000022273546,0.00025016067,0.000012315722,0.00040035913],"genre_scores_gemma":[0.99822897,0.00005326888,0.00018847763,0.00001219063,0.0000073420915,0.0000037338505,0.0011970751,0.0000062679014,0.00030268574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999552,0.0000025177876,0.000002357952,0.000013495749,0.000016386237,0.000010057176],"domain_scores_gemma":[0.9997583,0.00002079739,0.00008413846,0.00001650563,0.000032703072,0.00008762744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014152413,0.00021651183,0.00022766725,0.0006146863,0.00029298823,0.0004363136,0.00019080516,0.00015311659,0.0012521639],"category_scores_gemma":[0.0002537869,0.00010309789,0.0001826682,0.0003557059,0.00012665779,0.00013972104,0.00030455756,0.00021541023,0.0004068505],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042904113,0.000078210265,0.8657007,0.000064080385,0.00007936277,0.0011245434,0.00020663143,0.0011507744,0.12123791,0.00029157757,0.0004881455,0.009149112],"study_design_scores_gemma":[0.0000021065105,0.00004218819,0.9969175,0.0000028153622,0.000008980336,0.00025882391,0.000054203723,0.00066230586,0.0016165347,0.00003582108,0.00039569577,0.0000029725263],"about_ca_topic_score_codex":0.003141347,"about_ca_topic_score_gemma":0.0044177403,"teacher_disagreement_score":0.003141347,"about_ca_system_score_codex":0.00018604314,"about_ca_system_score_gemma":0.00010259596,"threshold_uncertainty_score":0.00624609},"labels":[],"label_agreement":null},{"id":"W4223937698","doi":"10.3847/1538-4357/ac6750","title":"Stellar Halos from the The Dragonfly Edge-on Galaxies Survey","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Halo; Stellar mass; Spiral galaxy; Astronomy; Disc; Galaxy; Elliptical galaxy; Star formation","score_opus":0.013071594152225965,"score_gpt":0.21242460891187417,"score_spread":0.1993530147596482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4223937698","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976799,0.000047791284,0.00004108335,0.000015545937,9.5305813e-7,0.0000029254386,0.0014143032,0.000011282041,0.0007862967],"genre_scores_gemma":[0.9942913,0.000037225836,0.00016403802,0.000016902035,0.0000033979902,0.0000032749692,0.0049397065,0.0000052294395,0.0005389572],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998981,0.0000123240025,0.0000031024274,0.000027245687,0.00002366273,0.000035510817],"domain_scores_gemma":[0.99962497,0.00004095634,0.00008160248,0.00004143185,0.000044064625,0.00016691258],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019776176,0.00022362737,0.00013875794,0.0013452235,0.0002751705,0.0004007625,0.00017426893,0.00015362698,0.0012509288],"category_scores_gemma":[0.0003465548,0.0000936461,0.0001519452,0.00062360516,0.0001877387,0.00018211726,0.00070615724,0.00012215362,0.00022990468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013602045,0.000023458928,0.9887285,0.000014164141,0.00005703883,0.000107720225,0.00034925895,0.0005086517,0.0029591864,0.00012373009,0.0016673442,0.0053250343],"study_design_scores_gemma":[0.0000045018746,0.00001484366,0.9981358,0.0000037638035,0.000007944253,0.00003556645,0.00013733465,0.00021640686,0.00036389055,0.000018977022,0.0010580457,0.00000293625],"about_ca_topic_score_codex":0.022056654,"about_ca_topic_score_gemma":0.054307543,"teacher_disagreement_score":0.022056654,"about_ca_system_score_codex":0.00046045557,"about_ca_system_score_gemma":0.00015904925,"threshold_uncertainty_score":0.0438565},"labels":[],"label_agreement":null},{"id":"W4223963220","doi":"10.3847/1538-4357/ac7b22","title":"Light from the Darkness: Detecting Ultra-diffuse Galaxies in the Perseus Cluster through Over-densities of Globular Clusters with a Log-Gaussian Cox Process","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Statistical Methods and Models","field":"Mathematics","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"St. Michael's Hospital; Canadian Institute for Theoretical Astrophysics; Ontario Power Generation; McMaster University; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Globular cluster; Physics; Astrophysics; Galaxy; Astronomy; Galaxy cluster; Cluster (spacecraft); Computer science","score_opus":0.035362766119521286,"score_gpt":0.3286058773434951,"score_spread":0.29324311122397384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4223963220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8983643,0.00014547816,0.09983255,0.00021723118,0.000011465814,0.000023013357,0.00013388011,0.00016469327,0.0011073656],"genre_scores_gemma":[0.99079096,0.000030427582,0.008794604,0.00001747296,0.000009778651,0.0000052046225,0.00006371661,0.000006655512,0.0002811188],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997483,0.000112259644,0.000006801178,0.000055289474,0.000054929304,0.000022448332],"domain_scores_gemma":[0.9962153,0.0025572162,0.0005599399,0.00031051412,0.00019469003,0.00016235994],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014429126,0.00023454113,0.00018005563,0.000851381,0.00020975085,0.00058476,0.00056833396,0.0002480919,0.00072357],"category_scores_gemma":[0.004012566,0.0001221606,0.00020358687,0.00043976473,0.0008350592,0.00048927846,0.0006357091,0.00035749868,0.000071386465],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007542235,0.00011269536,0.70169485,0.00008641163,0.00019591222,0.00060468726,0.00041336924,0.19429275,0.012251226,0.020890802,0.0010033542,0.067699775],"study_design_scores_gemma":[0.000023936078,0.000058795355,0.07342697,0.000008007519,0.000026806778,0.00016523898,0.000102942155,0.91374785,0.00317476,0.008872311,0.00036833374,0.000024156205],"about_ca_topic_score_codex":0.0069607627,"about_ca_topic_score_gemma":0.00591867,"teacher_disagreement_score":0.0069607627,"about_ca_system_score_codex":0.00057787856,"about_ca_system_score_gemma":0.00034062154,"threshold_uncertainty_score":0.013840497},"labels":[],"label_agreement":null},{"id":"W4223973071","doi":"10.3847/1538-4357/ac67a1","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Evidence for a Molecular Jet Launched at an Unprecedented Early Phase of Protostellar Evolution","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Science and Technology; Jet Propulsion Laboratory; National Research Foundation; National Natural Science Foundation of China; Agencia Estatal de Investigación; Japan Society for the Promotion of Science; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; California Institute of Technology; National Research Foundation of Korea","keywords":"Protostar; Physics; Astrophysics; Outflow; Submillimeter Array; Astronomy; Jet (fluid); Hydrostatic equilibrium; Star formation; Stars","score_opus":0.044497701137013554,"score_gpt":0.3178055133433895,"score_spread":0.27330781220637596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4223973071","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988881,0.00010268111,0.000053150296,0.000020370073,0.0000027626165,0.000005233923,0.00038260696,0.000021682796,0.00052357005],"genre_scores_gemma":[0.998216,0.00006533417,0.00031464896,0.000030417423,0.000013047011,0.000009131564,0.001017149,0.0000075292132,0.00032666526],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989974,0.000005752054,0.0000061986043,0.00003413439,0.000024445848,0.000029675937],"domain_scores_gemma":[0.9997223,0.000018698485,0.00010086465,0.000024995697,0.000029178542,0.000103960505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001679292,0.00023579787,0.00018215494,0.0014979452,0.00035104816,0.0004055821,0.00031606696,0.00023594566,0.0008591585],"category_scores_gemma":[0.00019450502,0.00013673039,0.00013135756,0.00057205185,0.00018041654,0.00019622101,0.0005363587,0.00016722915,0.0003494136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000096187185,0.000056552002,0.9551607,0.000034230132,0.000036957423,0.0006643613,0.0002601615,0.000044935314,0.03645018,0.00008660022,0.00058115914,0.0065278756],"study_design_scores_gemma":[0.0000050445774,0.000025765072,0.99802256,0.0000044356693,0.0000105548725,0.0002675999,0.00010479093,0.00009988774,0.0006528262,0.000020956804,0.0007832641,0.0000023263187],"about_ca_topic_score_codex":0.0044300305,"about_ca_topic_score_gemma":0.005910887,"teacher_disagreement_score":0.0044300305,"about_ca_system_score_codex":0.00021816301,"about_ca_system_score_gemma":0.00014354715,"threshold_uncertainty_score":0.008808494},"labels":[],"label_agreement":null},{"id":"W4224036210","doi":"10.3847/1538-4357/ac66d9","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): How Do Dense Core Properties Affect the Multiplicity of Protostars?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; Jet Propulsion Laboratory; Ministry of Science and Technology, Taiwan; Agencia Nacional de Investigación y Desarrollo; National Research Foundation of Korea; Agencia Estatal de Investigación; National Radio Astronomy Observatory; China Postdoctoral Science Foundation; Chinese Academy of Sciences; California Institute of Technology; Academia Sinica; Science and Technology Facilities Council; National Research Foundation; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Natural Science Foundation of China; National Science Foundation","keywords":"Physics; Protostar; Astrophysics; Orion Nebula; Molecular cloud; Stars; Star formation; Submillimeter Array; Protein filament; Millimeter; Astronomy","score_opus":0.034808862945480815,"score_gpt":0.25036075930499113,"score_spread":0.21555189635951033,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224036210","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991974,0.000149864,0.000053965552,0.000017293672,0.0000019909576,0.0000025807421,0.00030875424,0.0000057633174,0.00026243797],"genre_scores_gemma":[0.9993563,0.00004629447,0.00007500609,0.000008983009,0.0000049234714,0.0000019443023,0.0003935775,0.0000025661268,0.00011046536],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981123,0.00002553549,0.000012877722,0.00006349872,0.000041564563,0.000045259],"domain_scores_gemma":[0.99930334,0.000082241284,0.00026798857,0.000059717397,0.000101499725,0.00018521115],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031521774,0.00018674853,0.00020050629,0.0011893519,0.00033237605,0.0005317093,0.00030875576,0.00019908533,0.0005834152],"category_scores_gemma":[0.0007227734,0.00012480108,0.00015609468,0.0006967421,0.00016999863,0.000369238,0.0005283633,0.00014449749,0.00018709234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000022692262,0.000009429818,0.995743,0.000007448439,0.000022328863,0.00003949837,0.000085462,0.000039742725,0.0019067697,0.00002500392,0.00010447762,0.0019941158],"study_design_scores_gemma":[8.546793e-7,0.000006100669,0.99937505,0.0000019335935,0.0000052338783,0.000032142674,0.000077508805,0.0001716405,0.00013247813,0.000008810443,0.00018712546,0.0000010576935],"about_ca_topic_score_codex":0.009884768,"about_ca_topic_score_gemma":0.012258509,"teacher_disagreement_score":0.009884768,"about_ca_system_score_codex":0.00029691262,"about_ca_system_score_gemma":0.00014435343,"threshold_uncertainty_score":0.019654453},"labels":[],"label_agreement":null},{"id":"W4224062860","doi":"10.3847/1538-4357/ac5632","title":"Dissecting the Different Components of the Modest Accretion Bursts of the Very Young Protostar HOPS 373","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Instituto de Astrofísica de Andalucía; National Institutes of Natural Sciences; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Astronomical Observatory of Japan; Agencia Nacional de Investigación y Desarrollo; National Research Foundation of Korea; Chinese Academy of Sciences; California Institute of Technology; Academia Sinica; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Science Council; Science and Technology Facilities Council; National Research Foundation; Ministerio de Ciencia, Innovación y Universidades; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Natural Science Foundation of China; Agencia Estatal de Investigación; National Radio Astronomy Observatory; National Science Foundation","keywords":"Astrophysics; Outflow; Protostar; Physics; Brightness; Accretion (finance); Emission spectrum; Astronomy; Infrared; Bipolar outflow; Star formation; Spectral line; Galaxy","score_opus":0.01270932435073075,"score_gpt":0.22664744583863844,"score_spread":0.2139381214879077,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224062860","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994667,0.000026462852,0.00005615826,0.00000609414,6.748355e-7,0.0000016833786,0.000071550545,0.000005036695,0.00036554012],"genre_scores_gemma":[0.9994399,0.000023864115,0.000102521524,0.000007652071,0.000002266562,0.0000021927897,0.00017657495,0.0000045681704,0.00024045564],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999701,0.0000016644649,0.000002021889,0.000009246,0.000006402416,0.0000105590725],"domain_scores_gemma":[0.99987876,0.000015731399,0.000036048015,0.0000071120917,0.000013054755,0.000049285896],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000057564906,0.000117221876,0.0001274082,0.00056129816,0.0002852029,0.0003467886,0.00013148926,0.00015966936,0.00076668867],"category_scores_gemma":[0.00016139937,0.00010452564,0.00011817212,0.00029919815,0.00016008753,0.00014733059,0.00030287492,0.00014805007,0.00024543452],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004034913,0.000042898886,0.7387184,0.000035542587,0.000035560082,0.0019886598,0.00080913235,0.00034788137,0.24745622,0.00021932194,0.00023111678,0.009711941],"study_design_scores_gemma":[0.0000028043905,0.000046764235,0.995494,0.0000033729286,0.000006931963,0.00040906115,0.00024256282,0.00028448342,0.003093118,0.00006441664,0.00034874358,0.0000037645182],"about_ca_topic_score_codex":0.003217345,"about_ca_topic_score_gemma":0.007230043,"teacher_disagreement_score":0.003217345,"about_ca_system_score_codex":0.00025541766,"about_ca_system_score_gemma":0.00009831704,"threshold_uncertainty_score":0.0063972473},"labels":[],"label_agreement":null},{"id":"W4224072840","doi":"10.3847/1538-4357/ac66e7","title":"WO-type Wolf–Rayet Stars: The Last Hurrah of Massive Star Evolution*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Space Telescope Science Institute; National Science Foundation","keywords":"Astrophysics; Physics; Stars; Type (biology); Star (game theory); Line (geometry); Radiative transfer; Spectral line; Lambda; Wolf–Rayet star; Astronomy; Biology; Optics; Geometry; Mathematics","score_opus":0.010285944832674717,"score_gpt":0.2184933961543979,"score_spread":0.20820745132172316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224072840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965718,0.00019046085,0.001260425,0.00015634538,0.000012163244,0.0000058280016,0.00008595991,0.000029300352,0.0016878162],"genre_scores_gemma":[0.9993979,0.000031378957,0.00022522247,0.000016785536,0.0000073890496,0.0000025251347,0.00006173609,0.000008989777,0.00024801824],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998758,0.000026857853,0.000008174934,0.000038253318,0.000024387884,0.000026416586],"domain_scores_gemma":[0.99966216,0.00004101556,0.00010536827,0.000045045057,0.000046302765,0.00010010777],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003839453,0.00037391644,0.00040682548,0.0003908391,0.0004622463,0.0011086694,0.00054842356,0.00069971115,0.001206176],"category_scores_gemma":[0.0009068582,0.00021040885,0.00048933184,0.0003261577,0.00055110623,0.00072546914,0.00061943854,0.0003281432,0.0003273901],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054195,0.00013558056,0.8863789,0.0000860546,0.00017195505,0.001349311,0.0001786238,0.05615569,0.033021998,0.0061554024,0.0008154789,0.015009106],"study_design_scores_gemma":[0.000093139766,0.0003228128,0.6774933,0.000051272982,0.00008113265,0.00075392687,0.00042487387,0.30395028,0.0074330517,0.00642935,0.0028960817,0.00007072312],"about_ca_topic_score_codex":0.0022184744,"about_ca_topic_score_gemma":0.0016276505,"teacher_disagreement_score":0.0022184744,"about_ca_system_score_codex":0.0006579373,"about_ca_system_score_gemma":0.00015668671,"threshold_uncertainty_score":0.004773617},"labels":[],"label_agreement":null},{"id":"W4224119764","doi":"10.3847/1538-4357/ac532b","title":"Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO–Virgo Run O3b","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; University of British Columbia","funders":"Division of Human Resource Development; Govern de les Illes Balears; Agencia Estatal de Investigación; Great Southern Development Commission, Government of Western Australia; Japan Society for the Promotion of Science; Australian Research Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, India; Conseil Régional, Île-de-France; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; Kavli Foundation; U.S. Department of Energy; National Research, Development and Innovation Office; Korea Institute of Science and Technology Information; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Institute for Cosmic Ray Research, University of Tokyo; Council of Scientific and Industrial Research, India; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Ministerio de Ciencia e Innovación; Leverhulme Trust; European Commission; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Centres de Recerca de Catalunya; Institut des Origines de Lyon; Russian Science Foundation; Scottish Funding Council; European Social Fund; Royal Society; Science and Engineering Research Board; National Science Foundation","keywords":"LIGO; Physics; Gravitational wave; Neutron star; Gamma-ray burst; Astrophysics; Fermi Gamma-ray Space Telescope; Population; Astronomy; Luminosity; Galaxy","score_opus":0.008463117230327975,"score_gpt":0.22254908963974304,"score_spread":0.21408597240941507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224119764","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993624,0.000024480336,0.00017619944,0.000012786164,0.0000010661931,0.0000045141737,0.00018910074,0.000016955966,0.00021251722],"genre_scores_gemma":[0.9984503,0.00001522082,0.00045030224,0.000013421968,0.00000338657,0.0000047790136,0.00094932166,0.000008576937,0.00010468768],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995011,0.00008664871,0.000031216565,0.00009658565,0.00014666498,0.0001377141],"domain_scores_gemma":[0.99726665,0.00064582354,0.0010069519,0.00021694586,0.00016415822,0.00069946283],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009563508,0.0003099993,0.00040503405,0.0025143882,0.00066824746,0.00083507283,0.0003444287,0.00044863173,0.0010617605],"category_scores_gemma":[0.0017346942,0.00015299473,0.0005986539,0.0013024253,0.00038887325,0.00028395347,0.0008590942,0.00034308733,0.00026560863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003305208,0.00005986696,0.98762333,0.000009373819,0.000111551235,0.00012694196,0.00011408133,0.00038646473,0.007268514,0.000088080764,0.00015987454,0.0037213513],"study_design_scores_gemma":[0.00001264174,0.00006425818,0.99678254,0.000004281589,0.000029722472,0.00011806046,0.00011089748,0.0011726326,0.0014531257,0.000049082508,0.0001947628,0.00000802501],"about_ca_topic_score_codex":0.008224476,"about_ca_topic_score_gemma":0.02101847,"teacher_disagreement_score":0.008224476,"about_ca_system_score_codex":0.0004051802,"about_ca_system_score_gemma":0.000423869,"threshold_uncertainty_score":0.01635325},"labels":[],"label_agreement":null},{"id":"W4224136115","doi":"10.3847/1538-4357/ac9053","title":"Direct Optimal Mapping for 21 cm Cosmology: A Demonstration with the Hydrogen Epoch of Reionization Array","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Australian Research Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Massachusetts Institute of Technology; Newton Fund; National Science Foundation; Royal Society; Canadian Institute for Advanced Research; FP7 International Cooperation; Science and Technology Facilities Council; National Research Foundation; UK Research and Innovation; American Academy of Periodontology Foundation; McGill University; Gordon and Betty Moore Foundation","keywords":"Reionization; Physics; Cosmology; Epoch (astronomy); Astronomy; Astrophysics; Galaxy; Redshift","score_opus":0.010441583064015632,"score_gpt":0.21074418441105947,"score_spread":0.20030260134704383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224136115","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.25844392,0.00020110473,0.71930087,0.00084342196,0.00008885846,0.00006631725,0.00035082424,0.0065526753,0.014152058],"genre_scores_gemma":[0.68467253,0.000049668623,0.31342092,0.00011298917,0.000023703857,0.000037990478,0.00023327817,0.00023648719,0.0012124806],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996767,0.00010704475,0.000013221283,0.000050018516,0.00010565437,0.000047312522],"domain_scores_gemma":[0.99931073,0.00033215122,0.000040649993,0.00016647545,0.00010533585,0.000044710603],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008805047,0.00026347584,0.0002177642,0.0002358631,0.00022905703,0.00058156764,0.0006678979,0.0004294084,0.003109184],"category_scores_gemma":[0.0033329448,0.0001433182,0.00021660229,0.00034047707,0.00032545815,0.000650129,0.0009370427,0.00034833915,0.00072989136],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008789406,0.00033923527,0.024583828,0.000111053945,0.000106801985,0.0007368353,0.0005675135,0.35888118,0.054406468,0.05532857,0.012767782,0.4912918],"study_design_scores_gemma":[0.00007109521,0.00006850089,0.004138573,0.000008793545,0.000006424666,0.00016615797,0.000076082746,0.9533392,0.014138407,0.020901686,0.007063913,0.000021068643],"about_ca_topic_score_codex":0.002047099,"about_ca_topic_score_gemma":0.0019275814,"teacher_disagreement_score":0.003109184,"about_ca_system_score_codex":0.00025170654,"about_ca_system_score_gemma":0.00049519056,"threshold_uncertainty_score":0.010401249},"labels":[],"label_agreement":null},{"id":"W4224238386","doi":"10.3847/1538-4357/ac5cc5","title":"A Comparative Analysis to Deal with Missing Spectral Information Caused by RFI in Cosmological H i 21 cm Observations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Missing data; Theoretical physics; Physics; Astrophysics; Statistical physics; Econometrics; Mathematics; Statistics","score_opus":0.020483780549166376,"score_gpt":0.24669246656753369,"score_spread":0.2262086860183673,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224238386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7959534,0.0011050374,0.19786088,0.00044536105,0.00008385402,0.000071221584,0.00036539845,0.0021221768,0.0019925397],"genre_scores_gemma":[0.832862,0.00018314915,0.16465531,0.00015562995,0.000058126996,0.00003659718,0.0011870906,0.00020306607,0.000659088],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99862516,0.00055211113,0.000076437296,0.0002010433,0.00042670354,0.00011863806],"domain_scores_gemma":[0.99079216,0.005803967,0.00067977037,0.0009900028,0.0015081179,0.00022604871],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0044603795,0.0007916842,0.00051263964,0.0015640141,0.0005781915,0.00076815306,0.00090539514,0.0011735533,0.00066583365],"category_scores_gemma":[0.013747247,0.00027930306,0.00092769915,0.0007949766,0.0005184643,0.00094931334,0.00076805794,0.00059265544,0.00031202476],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0029999807,0.00052124297,0.102967486,0.0004908209,0.0011399128,0.0005969712,0.00062219735,0.4894069,0.056973927,0.0035905584,0.0037786325,0.33691132],"study_design_scores_gemma":[0.00007924011,0.0002900919,0.06660537,0.000032009728,0.0002093213,0.00021555516,0.00019191319,0.9044864,0.025191594,0.0010556112,0.0015828221,0.000059947084],"about_ca_topic_score_codex":0.0061806263,"about_ca_topic_score_gemma":0.0071131396,"teacher_disagreement_score":0.0061806263,"about_ca_system_score_codex":0.00045375217,"about_ca_system_score_gemma":0.0006680758,"threshold_uncertainty_score":0.023589015},"labels":[],"label_agreement":null},{"id":"W4224248644","doi":"10.3847/1538-4357/ac6d56","title":"CLASSY III. The Properties of Starburst-driven Warm Ionized Outflows*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Space Telescope Science Institute; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Redshift; Galaxy; Outflow; Kinetic energy; Interstellar medium; Supernova; Star formation; Spectral line; Ionization; Astronomy; Ion","score_opus":0.011874761353239118,"score_gpt":0.20100367555424042,"score_spread":0.1891289142010013,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224248644","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99878544,0.00005009727,0.00012257275,0.000004976976,0.0000013469418,0.000002790143,0.0006584016,0.0000072994085,0.00036720416],"genre_scores_gemma":[0.99799687,0.000025147183,0.000121541976,0.000007794225,0.0000045921547,0.00000441568,0.0015931417,0.0000052968207,0.00024099994],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977463,0.000016214102,0.000017047745,0.00007581571,0.00003685233,0.000079495876],"domain_scores_gemma":[0.99855,0.00016230119,0.00074143417,0.00012486432,0.00013727677,0.00028407483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000341156,0.00021495784,0.00023727123,0.0011327567,0.00034942126,0.0006889133,0.00019827322,0.00018583021,0.0019064195],"category_scores_gemma":[0.0007575019,0.00010951882,0.000263744,0.0006419852,0.00025754143,0.0003395995,0.00063306955,0.00017655312,0.00043373316],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042740376,0.00001122897,0.9956391,0.000005482697,0.000014104149,0.000019055817,0.00005300481,0.000055883313,0.0020905822,0.0000252463,0.00007333921,0.001970165],"study_design_scores_gemma":[0.0000010510383,0.0000093626495,0.99938023,0.0000010981644,0.0000024268093,0.000034609162,0.000046822668,0.00011787596,0.00025686686,0.000010477723,0.00013839535,7.920643e-7],"about_ca_topic_score_codex":0.0061904113,"about_ca_topic_score_gemma":0.0056267,"teacher_disagreement_score":0.0061904113,"about_ca_system_score_codex":0.00022196957,"about_ca_system_score_gemma":0.00013948038,"threshold_uncertainty_score":0.012308776},"labels":[],"label_agreement":null},{"id":"W4224264358","doi":"10.3847/1538-4357/ac5913","title":"The Central 1000 au of a Prestellar Core Revealed with ALMA. II. Almost Complete Freeze-out","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":76,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McMaster University","funders":"","keywords":"Physics; Astrophysics; Radiative transfer; Isotopologue; Protoplanetary disk; RADIUS; Astrochemistry; Planet; Young stellar object; Star formation; Stars; Molecule; Interstellar medium; Galaxy","score_opus":0.016028153232697222,"score_gpt":0.2289650969903748,"score_spread":0.21293694375767758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224264358","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929334,0.0002039577,0.00087619654,0.000065915716,0.0000130011185,0.000014338157,0.0005670224,0.00015609416,0.0051700408],"genre_scores_gemma":[0.99825853,0.000019871517,0.0005320053,0.000033330743,0.0000052532796,0.0000037596312,0.0002906138,0.000007676914,0.0008489712],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99997914,0.000001174926,7.2649755e-7,0.0000079000165,0.000004460879,0.000006618246],"domain_scores_gemma":[0.9999578,0.000004731939,0.000010205628,0.000006386854,0.0000059301124,0.000014897811],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000040621875,0.00015650096,0.0000750648,0.00028786284,0.0002502729,0.00021353584,0.00019189001,0.00031934117,0.0016830299],"category_scores_gemma":[0.000069217276,0.000094544805,0.00015121889,0.00009854541,0.00011255681,0.0001118401,0.00021751395,0.0001620832,0.0003692744],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066606555,0.0001268849,0.29449722,0.00007229835,0.000090523026,0.012650651,0.0004946606,0.0017794326,0.66109824,0.00082924595,0.0019335187,0.025761252],"study_design_scores_gemma":[0.000013222799,0.0001405272,0.963457,0.000008507379,0.000026753592,0.003327929,0.00014554481,0.005533311,0.021775257,0.00028394748,0.005279714,0.000008423539],"about_ca_topic_score_codex":0.0030096895,"about_ca_topic_score_gemma":0.004054671,"teacher_disagreement_score":0.0030096895,"about_ca_system_score_codex":0.00024503795,"about_ca_system_score_gemma":0.00007211557,"threshold_uncertainty_score":0.0059843063},"labels":[],"label_agreement":null},{"id":"W4224271516","doi":"10.3847/1538-4357/ac6bfd","title":"Substructures in Protoplanetary Disks Imprinted by Compact Planetary Systems","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Fondo Nacional de Desarrollo Científico y Tecnológico","keywords":"Planet; Physics; Neptune; Vortex; Protoplanetary disk; Astrophysics; Astronomy; Mechanics","score_opus":0.006168896471591681,"score_gpt":0.20326200866405697,"score_spread":0.19709311219246528,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224271516","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99940455,0.00002584875,0.00016930964,0.00001488406,0.0000020939056,0.000002141963,0.000023750434,0.000011334194,0.00034610325],"genre_scores_gemma":[0.99986696,0.0000070792894,0.00006967054,0.0000023622365,8.8048205e-7,0.0000010300673,0.000018666393,0.0000021830747,0.000031199863],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999335,0.000010902762,0.0000049390196,0.000015861971,0.00001146633,0.000023421826],"domain_scores_gemma":[0.99961036,0.00009692214,0.000112431,0.00006316462,0.000030670748,0.0000864312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001667561,0.00021645735,0.00024223446,0.0003703331,0.0005092507,0.00077392015,0.00033917712,0.00038251645,0.0013561617],"category_scores_gemma":[0.00096385216,0.0001893287,0.00029474404,0.00021887849,0.0006243054,0.000713525,0.00068203115,0.00027303176,0.00012896406],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008976562,0.00043923076,0.36836246,0.00014306669,0.00036929853,0.0020350413,0.0012159055,0.53749573,0.07118433,0.0048441943,0.00096916774,0.012043897],"study_design_scores_gemma":[0.00014434574,0.0005389721,0.25735855,0.0000387121,0.00009750337,0.00034103496,0.0010266675,0.72888064,0.0074092452,0.0031421522,0.000982599,0.000039477585],"about_ca_topic_score_codex":0.0037364583,"about_ca_topic_score_gemma":0.0024076686,"teacher_disagreement_score":0.0037364583,"about_ca_system_score_codex":0.00048902526,"about_ca_system_score_gemma":0.00016994741,"threshold_uncertainty_score":0.007429421},"labels":[],"label_agreement":null},{"id":"W4224305022","doi":"10.3847/1538-4357/ac67ee","title":"Metallicity of Galactic RR Lyrae from Optical and Infrared Light Curves. II. Period–Fourier–Metallicity Relations for First Overtone RR Lyrae","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Planetary Science Division; National Astronomical Observatories, Chinese Academy of Sciences; Jet Propulsion Laboratory; Max-Planck-Institut für Astronomie; Peking University; Max-Planck-Gesellschaft; Chinese Academy of Sciences; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Center for Cosmology and Astroparticle Physics, Ohio State University; Villum Fonden; Universität Basel; National Development and Reform Commission; Fermilab; National Science Foundation; Case Western Reserve University; University of Pittsburgh; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Princeton University; Johns Hopkins University; Ohio State University; Chinese Academy of Sciences South America Center for Astronomy; California Institute of Technology; U.S. Naval Observatory; U.S. Department of Energy; Gordon and Betty Moore Foundation; Drexel University; National Aeronautics and Space Administration","keywords":"RR Lyrae variable; Metallicity; Globular cluster; Galactic halo; Infrared; Stars; Galaxy","score_opus":0.012034932093956735,"score_gpt":0.22396575864335766,"score_spread":0.21193082654940093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224305022","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9920574,0.0007022784,0.0014114782,0.00004294815,0.000006817935,0.000012727963,0.0012082752,0.00017610856,0.0043819393],"genre_scores_gemma":[0.99780124,0.00008277632,0.0006955488,0.000014815467,0.0000101707965,0.0000051868788,0.0011340503,0.000025669138,0.0002303943],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972755,0.0000260162,0.00002091272,0.00010916803,0.00006981192,0.000046597816],"domain_scores_gemma":[0.9988267,0.00018412239,0.0005216863,0.00018496328,0.00017305341,0.00010953383],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054308824,0.00039098907,0.00018997138,0.003093098,0.00021191446,0.0006350027,0.00037489497,0.00037752793,0.0011101104],"category_scores_gemma":[0.0013509291,0.00020815442,0.00026367413,0.00089147664,0.00028845543,0.0004304239,0.0005156118,0.00027974573,0.00092156226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000104382045,0.000022872862,0.9613357,0.00006193993,0.00006244991,0.000054570024,0.00017289935,0.0018390014,0.016268872,0.00029823376,0.00053477584,0.01924429],"study_design_scores_gemma":[0.0000039045594,0.000014638055,0.9957136,0.000007533272,0.000010504315,0.000044517852,0.000035258625,0.001799558,0.0015885982,0.000087951965,0.00068902585,0.0000048974703],"about_ca_topic_score_codex":0.0027648914,"about_ca_topic_score_gemma":0.0033080694,"teacher_disagreement_score":0.003093098,"about_ca_system_score_codex":0.0005135564,"about_ca_system_score_gemma":0.00009740402,"threshold_uncertainty_score":0.005497575},"labels":[],"label_agreement":null},{"id":"W4224440095","doi":"10.3847/1538-4357/ac5ea3","title":"Constraining Warm Dark Matter and Population III Stars with the Global 21 cm Signal","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Solar System Exploration Research Virtual Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Reionization; Star formation; Stars; Dark matter; Cold dark matter; Redshift; Halo; Dark Ages; Dark matter halo; Virial theorem; Population; Virial mass; Warm dark matter; Galaxy formation and evolution; Galaxy; Scalar field dark matter; Cosmology; Dark energy","score_opus":0.006666255123571162,"score_gpt":0.20719919656464592,"score_spread":0.20053294144107475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224440095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9657309,0.000107845655,0.03228856,0.00011924068,0.0000037726104,0.000008933325,0.00016501681,0.00010476551,0.001470972],"genre_scores_gemma":[0.9976094,0.000020236834,0.0021104608,0.000019456227,0.0000026335288,0.000003635247,0.00011365316,0.0000083018695,0.00011230208],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99952066,0.00017297131,0.000024746001,0.00013192614,0.00009226562,0.000057465],"domain_scores_gemma":[0.9958657,0.0026541376,0.00071238016,0.00040871566,0.00015452078,0.00020444008],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022348398,0.0006315666,0.0003277833,0.0007481442,0.0003689855,0.00086780655,0.00044838892,0.00063746306,0.0014362057],"category_scores_gemma":[0.0075106593,0.00030619404,0.0006598504,0.00033328639,0.0006970575,0.0008269492,0.001243378,0.00043700874,0.000149735],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004340208,0.000093831615,0.6411902,0.000091546724,0.00033870543,0.0002733281,0.00017168891,0.2929434,0.028315775,0.016640967,0.00045384114,0.01905265],"study_design_scores_gemma":[0.0000495164,0.00022949012,0.21018174,0.000066226414,0.00017473512,0.00027906714,0.00016055208,0.74472725,0.02029706,0.022559892,0.0011906489,0.00008381692],"about_ca_topic_score_codex":0.00507923,"about_ca_topic_score_gemma":0.0042002173,"teacher_disagreement_score":0.00507923,"about_ca_system_score_codex":0.00061717007,"about_ca_system_score_gemma":0.00046272948,"threshold_uncertainty_score":0.011819124},"labels":[],"label_agreement":null},{"id":"W4224526085","doi":"10.3847/1538-4357/ac69da","title":"Three-dimensional General-relativistic Simulations of Neutrino-driven Winds from Rotating Proto-neutron Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Neutron star; Neutrino; Astrophysics; Stars; Nuclear physics; Astronomy","score_opus":0.016840671044649036,"score_gpt":0.3006924949582479,"score_spread":0.28385182391359887,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224526085","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868527,0.00011162132,0.0030916044,0.0003072165,0.00006165632,0.000037294554,0.0007213247,0.00020591736,0.008610708],"genre_scores_gemma":[0.99616843,0.000075952776,0.001859973,0.00009247107,0.000017880746,0.000027715405,0.00060565723,0.00006542208,0.0010863352],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998155,0.00004801496,0.000009031196,0.000023526827,0.000037278936,0.00006662252],"domain_scores_gemma":[0.9991248,0.0003118677,0.00014454135,0.00006418077,0.00012548608,0.00022900854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004982461,0.0006264067,0.0006855338,0.0004522027,0.0007396572,0.00088037224,0.0012004685,0.001243801,0.0028421301],"category_scores_gemma":[0.0020034858,0.00047743268,0.0011484098,0.00058281416,0.0010437976,0.00041689706,0.00080925564,0.0010651652,0.00026613384],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020829098,0.000101845224,0.006129405,0.000026449121,0.0000594821,0.0001676192,0.00007773473,0.98879224,0.0013654918,0.0019302202,0.00037963077,0.0007616864],"study_design_scores_gemma":[0.00007071403,0.00005193223,0.0027640813,0.0000053576828,0.0000153508,0.000014057162,0.00005370812,0.99594575,0.0003430842,0.00048127034,0.00024293986,0.000011855778],"about_ca_topic_score_codex":0.040204026,"about_ca_topic_score_gemma":0.017033497,"teacher_disagreement_score":0.040204026,"about_ca_system_score_codex":0.0012104438,"about_ca_system_score_gemma":0.0010026686,"threshold_uncertainty_score":0.07994002},"labels":[],"label_agreement":null},{"id":"W4224875183","doi":"10.3847/1538-4357/ac63cf","title":"The Next Generation Virgo Cluster Survey. XXXIII. Stellar Population Gradients in the Virgo Cluster Core Globular Cluster System","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Japan Society for the Promotion of Science; National Aeronautics and Space Administration; Agence Nationale de la Recherche; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; U.S. Department of State","keywords":"Globular cluster; Virgo Cluster; Cluster (spacecraft); Physics; Astrophysics; Population; Astronomy; Galaxy cluster; Stars; Galaxy; Computer science; Medicine","score_opus":0.03382887568920143,"score_gpt":0.24372725879744125,"score_spread":0.20989838310823983,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224875183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.992739,0.0001946556,0.00009453846,0.00007583661,0.000002445667,0.000007893874,0.0053441543,0.000026302727,0.0015150097],"genre_scores_gemma":[0.99259734,0.000071659895,0.00026140056,0.00002791135,0.0000034596208,0.000006741991,0.006346139,0.000008175872,0.0006771323],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991715,0.000014534123,0.0000030712288,0.000021164193,0.000021323109,0.000022654085],"domain_scores_gemma":[0.99984753,0.000017950875,0.00004045678,0.000018070492,0.000033070504,0.000042979893],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020284999,0.00011379855,0.00011806096,0.00082550215,0.00019618377,0.00040259288,0.0002003878,0.00020990551,0.0010315354],"category_scores_gemma":[0.0003892907,0.00007368586,0.0002096321,0.00084207766,0.00009429045,0.00016833369,0.0003977271,0.00013559964,0.0003378182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060073635,0.000018536843,0.9895822,0.000017137141,0.000057768062,0.00006438479,0.00011133578,0.0021200196,0.0014522405,0.00032145184,0.0016999508,0.0044950163],"study_design_scores_gemma":[0.0000017427386,0.0000045151537,0.9971545,0.0000028078387,0.0000047466024,0.00001748488,0.000046806334,0.0015550744,0.00009649858,0.000036552196,0.0010775928,0.0000017262815],"about_ca_topic_score_codex":0.07151302,"about_ca_topic_score_gemma":0.10612332,"teacher_disagreement_score":0.07151302,"about_ca_system_score_codex":0.0006393587,"about_ca_system_score_gemma":0.00021526137,"threshold_uncertainty_score":0.14219356},"labels":[],"label_agreement":null},{"id":"W4224903049","doi":"10.3847/1538-4357/ac6586","title":"Two Rings and a Marginally Resolved, 5 au Disk around LkCa 15 Identified via Near-infrared Sparse Aperture Masking Interferometry","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Eidgenössische Technische Hochschule Zürich; Office National d'études et de Recherches Aérospatiales; Max-Planck-Institut für Astronomie; Agence Nationale de la Recherche; Centre National de la Recherche Scientifique; Natural Sciences and Engineering Research Council of Canada; European Commission","keywords":"Physics; Astrophysics; Planet; Interferometry; Surface brightness; Planetary system; Brightness; Debris disk; Very Large Telescope; Stars; Astronomy; Galaxy","score_opus":0.010455803457403197,"score_gpt":0.2345789356847924,"score_spread":0.22412313222738922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224903049","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99890053,0.000032034186,0.00040614247,0.000011947481,0.0000023936539,0.0000042971365,0.00011859022,0.000052738942,0.00047134812],"genre_scores_gemma":[0.9991379,0.000005147082,0.00068138324,0.0000046887244,0.0000019882832,0.0000020145692,0.00010770201,0.000004552597,0.00005454966],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999007,0.000007320379,0.0000049338023,0.000039520495,0.000019758221,0.000027752203],"domain_scores_gemma":[0.99973375,0.000042342523,0.00007722661,0.000052211846,0.00003126826,0.00006318489],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000138238,0.00018018515,0.00022673619,0.0005875973,0.00037952527,0.00043469682,0.00045772304,0.00030618935,0.0007805099],"category_scores_gemma":[0.00045519197,0.00013832067,0.00023170278,0.00025310763,0.00023108194,0.00022046546,0.00042824456,0.00014286098,0.00020371891],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007796743,0.00020970695,0.7788057,0.00010256945,0.00016190145,0.0032787544,0.0013712782,0.013149709,0.16825828,0.0018047853,0.0012040333,0.03087356],"study_design_scores_gemma":[0.000038438433,0.00016864561,0.9319298,0.000026386246,0.00009566755,0.0010288989,0.00051016617,0.055765193,0.007818825,0.00042763253,0.002162785,0.000027572598],"about_ca_topic_score_codex":0.0064093485,"about_ca_topic_score_gemma":0.010105845,"teacher_disagreement_score":0.0064093485,"about_ca_system_score_codex":0.00028639063,"about_ca_system_score_gemma":0.00024215526,"threshold_uncertainty_score":0.012744069},"labels":[],"label_agreement":null},{"id":"W4224911349","doi":"10.3847/1538-4357/ac63bc","title":"Effects of Magnetic Field Orientations in Dense Cores on Gas Kinematics in Protostellar Envelopes","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council","keywords":"Physics; Protostar; Astrophysics; Angular momentum; Magnetic field; Star formation; Envelope (radar); Rotation (mathematics); Molecular cloud; Specific relative angular momentum; Accretion (finance); Total angular momentum quantum number; Stars; Classical mechanics; Angular momentum coupling","score_opus":0.006221290928660421,"score_gpt":0.23378130348528525,"score_spread":0.22756001255662484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224911349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996538,0.00004326736,0.00011443076,0.000004509159,8.534205e-7,6.693235e-7,0.000033769353,0.000004970607,0.00014375133],"genre_scores_gemma":[0.9998969,0.000010688821,0.00003149791,0.0000015807232,7.7194505e-7,2.4000286e-7,0.00003792119,0.0000015159856,0.000018930612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986076,0.00003832106,0.000010228118,0.000033752454,0.00002793026,0.000029050796],"domain_scores_gemma":[0.99890184,0.00036512213,0.0004067242,0.00009873714,0.00007626126,0.00015133986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024804627,0.00015840419,0.00014984184,0.0004261398,0.00015966936,0.00047592417,0.00010220284,0.0000965782,0.00047197856],"category_scores_gemma":[0.00170503,0.00011515146,0.000098724304,0.0002702299,0.00028753342,0.00017506236,0.00029722587,0.000104034225,0.00009340913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002685164,0.000025001105,0.96644354,0.000011044758,0.000037318954,0.0001332118,0.000089435795,0.0033639877,0.025766458,0.00009826976,0.00004368824,0.0037195806],"study_design_scores_gemma":[0.0000024919686,0.000020861617,0.99673504,0.0000017064868,0.0000069025177,0.00003782284,0.000047403297,0.0015315935,0.0015196457,0.000030364563,0.00006441077,0.0000016277821],"about_ca_topic_score_codex":0.0030396986,"about_ca_topic_score_gemma":0.0028366838,"teacher_disagreement_score":0.0030396986,"about_ca_system_score_codex":0.0002805949,"about_ca_system_score_gemma":0.0001048105,"threshold_uncertainty_score":0.0060439706},"labels":[],"label_agreement":null},{"id":"W4224942125","doi":"10.3847/1538-4357/ac6c86","title":"A Multiwavelength Study of the Highly Asymmetrical Debris Disk around HD 111520","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Ministério da Ciência, Tecnologia e Inovação; European Space Agency; National Aeronautics and Space Administration; Ministerio de Ciencia, Tecnología e Innovación Productiva; National Science Foundation","keywords":"Debris disk; Physics; Asymmetry; Astrophysics; Brightness; Spectral energy distribution; Wavelength; Planet; Halo; Thin disk; Planetary system; Astronomy; Stars; Optics; Galaxy","score_opus":0.012850611059987202,"score_gpt":0.2393680199374665,"score_spread":0.22651740887747931,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224942125","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990274,0.000054085936,0.000118454824,0.0000130326225,0.0000026372693,0.0000029874373,0.00010465961,0.000009379601,0.0006675458],"genre_scores_gemma":[0.9994111,0.000016270604,0.00023791203,0.0000128998745,0.0000034706832,0.0000021725155,0.00016738419,0.0000030342012,0.00014573093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999361,0.0000057453612,0.000003698255,0.000022544767,0.000013208176,0.000018688985],"domain_scores_gemma":[0.99982685,0.000025130184,0.000048980455,0.000020759184,0.00002629678,0.000051913477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001260759,0.00020826996,0.00023131559,0.00063103595,0.0005332431,0.0004127373,0.00022964658,0.00021968028,0.00089172344],"category_scores_gemma":[0.00024155248,0.0002066856,0.00013113454,0.00031020388,0.00019182652,0.0002495093,0.00039416942,0.00018933376,0.00023549661],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046191696,0.00016593232,0.68109477,0.00008329083,0.00011243916,0.0025629355,0.00088859914,0.001027804,0.2996454,0.0002271253,0.00063958426,0.013090322],"study_design_scores_gemma":[0.0000051520165,0.00003556597,0.9972537,0.0000043227224,0.000009860304,0.00026533892,0.00014467671,0.00050984713,0.0013724528,0.000015651212,0.00037962222,0.000003869527],"about_ca_topic_score_codex":0.0037243033,"about_ca_topic_score_gemma":0.009339791,"teacher_disagreement_score":0.0037243033,"about_ca_system_score_codex":0.00038037155,"about_ca_system_score_gemma":0.000096712654,"threshold_uncertainty_score":0.007405281},"labels":[],"label_agreement":null},{"id":"W4224995062","doi":"10.3847/1538-4357/ac68f2","title":"The Effects of Disk-induced Apsidal Precession on Planets Captured into Mean Motion Resonance","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Exoplanet; Planet; Apsidal precession; Physics; Precession; Planetary migration; Population; Astrophysics; Mean motion; Astronomy; Perturbation (astronomy); Libration (molecule); Limiting; Planetesimal; Solar System; Celestial mechanics; Planetary system; Mathematics; Geometry","score_opus":0.006477933096398981,"score_gpt":0.2255464289761841,"score_spread":0.2190684958797851,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4224995062","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974825,0.00007144052,0.0010562121,0.000056412435,0.0000036001377,0.00000277497,0.000034250475,0.000033652046,0.0012591723],"genre_scores_gemma":[0.9997775,0.000017737773,0.00010293399,0.000003821541,9.18453e-7,0.0000010981944,0.000010121543,0.0000046952487,0.000081010156],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991345,0.00002598518,0.000005612191,0.000016105125,0.000015704829,0.0000231704],"domain_scores_gemma":[0.99844056,0.0010254513,0.00023823812,0.00012742824,0.00007306975,0.00009514908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022325643,0.00016276947,0.0002512443,0.0002686772,0.00031287284,0.0005496384,0.0003802458,0.00030197765,0.0016136318],"category_scores_gemma":[0.0035823835,0.00011911873,0.00022815574,0.00015234256,0.000534579,0.00037118583,0.0004906188,0.00037644777,0.0000918943],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010540932,0.0003343513,0.058408078,0.00023465464,0.00015726032,0.002111759,0.00048389798,0.7551309,0.1585097,0.010921779,0.0007244932,0.011929118],"study_design_scores_gemma":[0.00006502746,0.0004427243,0.04320475,0.000022787242,0.000053832082,0.00032626264,0.00027163594,0.92129457,0.031319592,0.002414931,0.00054710195,0.000036856007],"about_ca_topic_score_codex":0.0023186766,"about_ca_topic_score_gemma":0.0010651777,"teacher_disagreement_score":0.0023186766,"about_ca_system_score_codex":0.00048155445,"about_ca_system_score_gemma":0.00013340346,"threshold_uncertainty_score":0.005398214},"labels":[],"label_agreement":null},{"id":"W4225091474","doi":"10.3847/1538-4357/ac6a58","title":"The Host Galaxy of the Recoiling Black Hole Candidate in 3C 186: An Old Major Merger Remnant at the Center of a z = 1 Cluster","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Galaxy; Black hole (networking); Astronomy; Supermassive black hole; Quasar; Galaxy merger; Galaxy formation and evolution","score_opus":0.0064572773515698696,"score_gpt":0.21087032838122072,"score_spread":0.20441305102965085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225091474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994783,0.000026672746,0.00009585368,0.000011796069,0.000001685374,0.0000022443671,0.000072155555,0.000011464062,0.000299857],"genre_scores_gemma":[0.9994881,0.0000108168615,0.00017547247,0.000008081785,0.0000034777959,9.182712e-7,0.00017843662,0.0000036622873,0.00013108298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999491,0.000002822529,0.000001581406,0.00001401769,0.000009923219,0.0000225875],"domain_scores_gemma":[0.99981827,0.000008505401,0.0000574455,0.000014560723,0.000016197082,0.000085024294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008686119,0.00023130368,0.00024910472,0.00068139774,0.0005072798,0.000509414,0.0002708172,0.00023771844,0.0008161904],"category_scores_gemma":[0.00013892262,0.00012454097,0.00019162617,0.00039618826,0.00031646737,0.00018066977,0.0004348999,0.0002035925,0.00027035875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042094247,0.00009853249,0.91465324,0.000030598963,0.000056501678,0.004465034,0.00061083207,0.0010449731,0.072579846,0.0004254266,0.0006200778,0.0049939533],"study_design_scores_gemma":[0.000007046274,0.00003601396,0.99529403,0.0000026333817,0.000015368461,0.0006605904,0.0001964885,0.0015057431,0.0018459231,0.00004708309,0.00038248143,0.0000065638355],"about_ca_topic_score_codex":0.0074058804,"about_ca_topic_score_gemma":0.008227464,"teacher_disagreement_score":0.0074058804,"about_ca_system_score_codex":0.00037085544,"about_ca_system_score_gemma":0.00014521033,"threshold_uncertainty_score":0.014725566},"labels":[],"label_agreement":null},{"id":"W4225152000","doi":"10.3847/1538-4357/ac6870","title":"A Near-infrared Look at AGN Feedback in Bulgeless Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Max-Planck-Gesellschaft; Chinese Academy of Sciences; Gordon and Betty Moore Foundation; Queen's University Belfast; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Universität Basel; Fermilab; National Science Foundation; Case Western Reserve University; University of Pittsburgh; Los Alamos National Laboratory; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Queen's University; Ohio State University; Durham University; Drexel University; U.S. Naval Observatory; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Space Telescope Science Institute; W. M. Keck Foundation","keywords":"Physics; Supermassive black hole; Astrophysics; Galaxy; Bulge; Population; Active galactic nucleus; Redshift; Astronomy; Virial theorem; Quasar; Medicine","score_opus":0.007046276247873766,"score_gpt":0.2024281984080724,"score_spread":0.19538192216019865,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225152000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904877,0.000085425614,0.000073408126,0.000019965655,0.0000013206835,0.0000014364349,0.00006497722,0.000007975846,0.00069670676],"genre_scores_gemma":[0.9995245,0.000031983753,0.00009027538,0.000019608677,0.0000044811845,0.0000012102262,0.00010400606,0.000002009936,0.00022184743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999269,0.000010531635,0.0000037207733,0.00001783942,0.000013900419,0.000027015858],"domain_scores_gemma":[0.999482,0.000106636246,0.00017895052,0.0000246458,0.000063109546,0.0001446362],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001861835,0.00012982455,0.00014630622,0.0014645786,0.00023828076,0.00038745784,0.000144737,0.00017441457,0.0017370038],"category_scores_gemma":[0.00041291324,0.000077936704,0.00011360816,0.00053640496,0.00021923981,0.00024544037,0.00032171063,0.00020705209,0.00020626627],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050074203,0.000031498417,0.98578805,0.0000100482675,0.00001577668,0.00014890917,0.00031945953,0.000042911975,0.009261945,0.000065000015,0.00008423757,0.004182109],"study_design_scores_gemma":[5.044532e-7,0.00001872616,0.99943894,0.0000015725822,0.000003272539,0.00007199744,0.00012473555,0.000037360332,0.00019032766,0.000017852799,0.00009385733,8.547771e-7],"about_ca_topic_score_codex":0.0017966451,"about_ca_topic_score_gemma":0.0033539203,"teacher_disagreement_score":0.0017966451,"about_ca_system_score_codex":0.00013874179,"about_ca_system_score_gemma":0.000045623547,"threshold_uncertainty_score":0.005810857},"labels":[],"label_agreement":null},{"id":"W4225268895","doi":"10.3847/1538-4357/ac61dc","title":"Discovery of PSR J0523-7125 as a Circularly Polarized Variable Radio Source in the Large Magellanic Cloud","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council; Ministero degli Affari Esteri e della Cooperazione Internazionale","keywords":"Pulsar; Physics; Astrophysics; Large Magellanic Cloud; Astronomy; Small Magellanic Cloud; Milky Way; Galaxy; Polarization (electrochemistry); Spectral index; Spectral line","score_opus":0.007354934432062041,"score_gpt":0.2726737855897613,"score_spread":0.26531885115769926,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225268895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987496,0.00022107629,0.00020597596,0.000046685345,0.000009914332,0.0000052980313,0.0000773782,0.000010412895,0.0006736672],"genre_scores_gemma":[0.9995121,0.000053421347,0.00012676774,0.000021857708,0.00000896823,0.0000017225456,0.00009348409,0.0000010226877,0.0001806337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998716,0.000010166613,0.000006277545,0.000034667253,0.00003678272,0.00004041391],"domain_scores_gemma":[0.9997696,0.00001652776,0.000064728425,0.000018095208,0.000025577101,0.0001053588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019674368,0.00019332707,0.0001906493,0.0011619831,0.00078702334,0.0007509667,0.00039179143,0.0003711575,0.0008333752],"category_scores_gemma":[0.00029586485,0.000109971435,0.00016758514,0.000798669,0.0003896596,0.00022151436,0.0005082311,0.00021777833,0.00023657727],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014898165,0.00008766386,0.88506603,0.000055174125,0.00008407042,0.016644102,0.00080707454,0.00038772894,0.07068563,0.0012279799,0.0011413743,0.023664266],"study_design_scores_gemma":[0.000009745225,0.00013969585,0.98091966,0.000018788569,0.000042032316,0.0070463023,0.00066053733,0.0006220893,0.004853082,0.00028247258,0.0053914185,0.000014216752],"about_ca_topic_score_codex":0.0038375496,"about_ca_topic_score_gemma":0.005073758,"teacher_disagreement_score":0.0038375496,"about_ca_system_score_codex":0.00036286653,"about_ca_system_score_gemma":0.00025466894,"threshold_uncertainty_score":0.007630408},"labels":[],"label_agreement":null},{"id":"W4225331299","doi":"10.3847/1538-4357/ac5cc0","title":"Observing Planet-driven Dust Spirals with ALMA","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"European Research Council; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; McMaster University; University of Victoria; Compute Canada; Alfred P. Sloan Foundation","keywords":"Planet; Physics; Astrophysics; Spiral galaxy; Radiative transfer; Submillimeter Array; Astronomy; Thermal; Star formation; Stars","score_opus":0.015649663568125857,"score_gpt":0.2251898163149981,"score_spread":0.20954015274687224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225331299","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97558403,0.000056491383,0.019280935,0.00009674952,0.00002036873,0.00004155942,0.00039670177,0.0016989984,0.0028242045],"genre_scores_gemma":[0.98050445,0.000010847392,0.01896905,0.000028218412,0.000010000828,0.000016491189,0.00021251506,0.000027100268,0.00022125545],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99990964,0.000016678225,0.0000032331968,0.00002887004,0.000025096984,0.000016383898],"domain_scores_gemma":[0.9996568,0.000115923496,0.00003266923,0.000084874795,0.000061052095,0.000048700836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002987683,0.0001350332,0.00017573552,0.00034297124,0.0001921641,0.0003874087,0.00043496705,0.00027686203,0.0012632194],"category_scores_gemma":[0.0006420561,0.00012918808,0.00020441315,0.00019387828,0.00012896,0.0003473468,0.0002990131,0.00017181269,0.00017359809],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00276288,0.000589142,0.3269886,0.00019136677,0.00030890436,0.00043290772,0.0004937506,0.044446155,0.50095516,0.0033779468,0.0030528556,0.11640032],"study_design_scores_gemma":[0.00027580347,0.0010646235,0.22578527,0.000021955242,0.000139661,0.00040029862,0.00016878592,0.64096737,0.11989181,0.0026686445,0.008549238,0.00006655134],"about_ca_topic_score_codex":0.0012747585,"about_ca_topic_score_gemma":0.0022786364,"teacher_disagreement_score":0.0012747585,"about_ca_system_score_codex":0.0002920598,"about_ca_system_score_gemma":0.000111775924,"threshold_uncertainty_score":0.0042259097},"labels":[],"label_agreement":null},{"id":"W4225386138","doi":"10.3847/1538-4357/ac5a4d","title":"A Multiwavelength Study of ELAN Environments (AMUSE<sup>2</sup>). Mass Budget, Satellites Spin Alignment, and Gas Infall in a Massive z ∼ 3 Quasar Host Halo","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; Science and Technology Facilities Council; National Research Foundation; University of Toronto; European Commission; Academia Sinica; Deutsche Forschungsgemeinschaft; National Radio Astronomy Observatory; Smithsonian Institution; Korea Astronomy and Space Science Institute; Fondazione Cariplo; National Science Foundation","keywords":"Physics; Astrophysics; Quasar; Galaxy; Halo; Redshift; Baryon; Star formation; Dark matter; Stellar mass","score_opus":0.007026325107896114,"score_gpt":0.21051078184148053,"score_spread":0.20348445673358442,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225386138","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999423,0.000028922526,0.000062598614,0.00001002847,5.183903e-7,0.0000017649468,0.00012463274,0.0000060276643,0.00034255558],"genre_scores_gemma":[0.9990145,0.000027192862,0.00035395002,0.000015255807,0.000005593974,0.0000032310975,0.00033308956,0.000006187007,0.00024089668],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999144,0.000016701768,0.0000044396384,0.000021161432,0.000016129181,0.000027187316],"domain_scores_gemma":[0.999795,0.000028434808,0.000074797026,0.000023898723,0.000023113853,0.00005468161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016024942,0.00018068889,0.0001335091,0.0009636717,0.00038406224,0.00034114913,0.00017397507,0.00012655264,0.0006660139],"category_scores_gemma":[0.00018340137,0.00012230923,0.0001524857,0.0005302216,0.00013195298,0.00022950911,0.0005814875,0.00016486662,0.00014133276],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024098081,0.00012059599,0.9367392,0.000015582982,0.000085543346,0.0015095496,0.00049842364,0.00045648072,0.05039551,0.00016267461,0.00038889993,0.009386608],"study_design_scores_gemma":[0.0000025120282,0.000027281556,0.99797326,8.817712e-7,0.000005972092,0.00029447814,0.00012736302,0.0002869428,0.00087012927,0.000017137088,0.00039175112,0.0000022981512],"about_ca_topic_score_codex":0.0032218504,"about_ca_topic_score_gemma":0.007374484,"teacher_disagreement_score":0.0032218504,"about_ca_system_score_codex":0.00025273263,"about_ca_system_score_gemma":0.000062593455,"threshold_uncertainty_score":0.006406188},"labels":[],"label_agreement":null},{"id":"W4225407867","doi":"10.3847/1538-4357/ac5048","title":"First Combined Study on Lorentz Invariance Violation from Observations of Energy-dependent Time Delays from Multiple-type Gamma-Ray Sources. I. Motivation, Method Description, and Validation through Simulations of H.E.S.S., MAGIC, and VERITAS Data Sets","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Noncommutative and Quantum Gravity Theories","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"European Regional Development Fund; Generalitat de Catalunya; European Commission; Ministerio de Ciencia e Innovación; Hrvatska Zaklada za Znanost; Centres de Recerca de Catalunya","keywords":"Physics; Redshift; Quantum gravity; Lorentz covariance; Cosmic distance ladder; Population; Photon; Theoretical physics; Statistical physics; Astrophysics; Galaxy; Lorentz transformation; Quantum; Quantum mechanics","score_opus":0.06224125450008888,"score_gpt":0.28851735761195174,"score_spread":0.22627610311186286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225407867","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9809818,0.00016367313,0.016242003,0.0001485839,0.000013979753,0.000054345557,0.0005469879,0.0001684521,0.0016800961],"genre_scores_gemma":[0.9849412,0.000066321656,0.013899237,0.000025537132,0.000012035355,0.000058497128,0.0007048443,0.00007821595,0.00021409545],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997253,0.0001197271,0.000016259693,0.000040114573,0.000072263334,0.00002638172],"domain_scores_gemma":[0.995523,0.0033964308,0.00036946184,0.00027559657,0.00030917232,0.00012643942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018209136,0.00037977606,0.00038703403,0.00055460836,0.00047261335,0.0006806666,0.0010758677,0.0005845226,0.0009386659],"category_scores_gemma":[0.0068429606,0.00028991228,0.00067495235,0.0006214651,0.0004207649,0.00067794556,0.0007785729,0.00070964673,0.000083936626],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030594895,0.0002964423,0.07165812,0.00019614748,0.00031292366,0.00038960978,0.00030041934,0.8984031,0.0066601126,0.0052661514,0.00081857643,0.015392527],"study_design_scores_gemma":[0.00007372983,0.00013608472,0.01218296,0.000019839896,0.000044980483,0.000058570746,0.000046024466,0.9835133,0.0024442163,0.0010421482,0.00041309002,0.000025080217],"about_ca_topic_score_codex":0.010016162,"about_ca_topic_score_gemma":0.008702075,"teacher_disagreement_score":0.010016162,"about_ca_system_score_codex":0.0007321101,"about_ca_system_score_gemma":0.00064922165,"threshold_uncertainty_score":0.01991576},"labels":[],"label_agreement":null},{"id":"W4225489403","doi":"10.3847/1538-4357/ac63b7","title":"Coevolution of Brightest Cluster Galaxies and Their Host Clusters in IllustrisTNG","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Sigma; Physics; Velocity dispersion; Redshift; Astrophysics; Scaling; Galaxy; Halo; Cluster (spacecraft); Astronomy; Geometry; Mathematics","score_opus":0.006238929000639644,"score_gpt":0.19303751896577465,"score_spread":0.18679858996513501,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225489403","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967077,0.000038163584,0.00052630925,0.00013212491,0.0000062028753,0.0000057248944,0.00020242843,0.00006347124,0.0023178388],"genre_scores_gemma":[0.99846894,0.000022203338,0.00062929984,0.00004591815,0.000004705558,0.00000633678,0.00033932982,0.000034317258,0.00044883066],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984837,0.000037221864,0.0000045974593,0.000036663492,0.00002019297,0.000052949927],"domain_scores_gemma":[0.99890554,0.00039089448,0.0001250189,0.00011015217,0.000112400376,0.0003559681],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007094111,0.00030589235,0.0005694279,0.00066222233,0.000890796,0.0012529745,0.001168364,0.00076142343,0.002800919],"category_scores_gemma":[0.00301839,0.0003576642,0.00061288255,0.0006283668,0.00078228506,0.00071777665,0.0009879599,0.00071722205,0.0002199064],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027998074,0.00015668393,0.13808437,0.000036617417,0.00019309726,0.00030185666,0.00036337395,0.8469993,0.0021622085,0.006146579,0.0021059152,0.0031699436],"study_design_scores_gemma":[0.000111416004,0.00007205649,0.035384208,0.000014015664,0.000051580937,0.000056902525,0.00018681904,0.96025,0.0007534949,0.0022017038,0.0008849265,0.000032936205],"about_ca_topic_score_codex":0.048783287,"about_ca_topic_score_gemma":0.035391606,"teacher_disagreement_score":0.048783287,"about_ca_system_score_codex":0.001740195,"about_ca_system_score_gemma":0.0005792842,"threshold_uncertainty_score":0.09699869},"labels":[],"label_agreement":null},{"id":"W4225725315","doi":"10.3847/1538-4357/ac6025","title":"Physical Properties of the Supernova Remnant Population in the Small Magellanic Cloud","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Large Magellanic Cloud; Supernova remnant; Astrophysics; Astronomy; Supernova; Near-Earth supernova; Small Magellanic Cloud; Population; Stars; Medicine","score_opus":0.01579550197561463,"score_gpt":0.20740024781313662,"score_spread":0.191604745837522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4225725315","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995183,0.00005219611,0.000112429865,0.0000041857384,5.110987e-7,0.0000024290964,0.00009473794,0.0000038042836,0.00021140576],"genre_scores_gemma":[0.9997004,0.00001751191,0.0000384615,0.0000011220867,9.918381e-7,8.5123384e-7,0.00018645554,0.0000016694839,0.000052518575],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998915,0.000015288038,0.000009982415,0.000025482506,0.000032471067,0.000025230149],"domain_scores_gemma":[0.9989274,0.000281764,0.00034101313,0.00007636853,0.00016931066,0.00020407714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005595299,0.00013560028,0.00017001857,0.0010772214,0.00019771725,0.00057001057,0.00033053537,0.00015545776,0.0011105821],"category_scores_gemma":[0.001968272,0.00009836711,0.00018577599,0.00046749046,0.00035556214,0.0002098765,0.00023745613,0.00011865596,0.00020841915],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013321449,0.000023568264,0.9846821,0.000009335383,0.000046288947,0.0001727462,0.000064879554,0.0014436417,0.011867704,0.00019081312,0.000036007776,0.0013296731],"study_design_scores_gemma":[0.0000053102704,0.000080890255,0.9940598,0.0000027287529,0.000012377567,0.00036608524,0.00008866359,0.0032708081,0.0018440624,0.00009786266,0.00016595374,0.000005577719],"about_ca_topic_score_codex":0.005130549,"about_ca_topic_score_gemma":0.0030526926,"teacher_disagreement_score":0.005130549,"about_ca_system_score_codex":0.00026900735,"about_ca_system_score_gemma":0.00013380146,"threshold_uncertainty_score":0.010201395},"labels":[],"label_agreement":null},{"id":"W4226087780","doi":"10.3847/1538-4357/ac4506","title":"Radio and X-Ray Observations of the Luminous Fast Blue Optical Transient AT 2020xnd","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; York University","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Office of Science; Korea Astronomy and Space Science Institute; Tata Institute of Fundamental Research; Commonwealth Scientific and Industrial Research Organisation; Northwestern University; York University; National Astronomical Observatory of Japan; New Mexico State University; Associated Universities; Heising-Simons Foundation; Carnegie Mellon University; University of Arizona; College of Engineering, Michigan State University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Canadian Institute for Advanced Research; U.S. Department of Energy; Smithsonian Institution; National Radio Astronomy Observatory; Harvard University; Australian Government; National Research Foundation; Ohio State University; National Aeronautics and Space Administration; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Astrophysics","score_opus":0.013042802525534095,"score_gpt":0.20593301873681388,"score_spread":0.19289021621127977,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226087780","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99391866,0.00013490708,0.00030411466,0.0000544343,0.000014821358,0.000009310693,0.0010520502,0.00006727324,0.0044444744],"genre_scores_gemma":[0.9938791,0.000082069215,0.00055733026,0.00008165241,0.000017017474,0.000012941693,0.0037579061,0.000022595847,0.0015892305],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993753,0.0000025357701,0.0000023478153,0.000013094539,0.000017412003,0.00002700074],"domain_scores_gemma":[0.99985766,0.0000095863315,0.00003358269,0.000012474313,0.000020780582,0.00006590704],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016979566,0.00024052199,0.00020858,0.00068246806,0.0003999151,0.00046189193,0.0002481953,0.0003109278,0.001621918],"category_scores_gemma":[0.00016208907,0.00015462,0.00018952215,0.00036200465,0.00018138022,0.00017885905,0.000630497,0.0004249221,0.0004937344],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021251147,0.0003606103,0.6392051,0.00015064665,0.0001184195,0.0049391203,0.0010030738,0.0016574223,0.3112485,0.0010946464,0.0049975454,0.033099767],"study_design_scores_gemma":[0.000017486056,0.00007782746,0.9923264,0.00000973719,0.000010943663,0.00034867608,0.0001413183,0.00045848894,0.0031943528,0.00005509139,0.0033532847,0.0000063099405],"about_ca_topic_score_codex":0.0048143105,"about_ca_topic_score_gemma":0.0074720536,"teacher_disagreement_score":0.0048143105,"about_ca_system_score_codex":0.00048116627,"about_ca_system_score_gemma":0.0001764323,"threshold_uncertainty_score":0.009572566},"labels":[],"label_agreement":null},{"id":"W4226092512","doi":"10.3847/1538-4357/ac616f","title":"The Complexity of the Cetus Stream Unveiled from the Fusion of STREAMFINDER and StarGO","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; University of Victoria","funders":"Agence Nationale de la Recherche","keywords":"Physics; Globular cluster; Astrophysics; Galaxy; Milky Way; Dwarf galaxy; Debris; Astronomy; Sky; Metallicity","score_opus":0.017874472223406615,"score_gpt":0.21812437207466437,"score_spread":0.20024989985125774,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226092512","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9881065,0.00019495908,0.0068092323,0.0001018379,0.000015683316,0.000020544736,0.0009316451,0.0010221547,0.0027974313],"genre_scores_gemma":[0.9887454,0.0000680989,0.009013122,0.00002884534,0.000016463047,0.000006153945,0.0015348045,0.00010086099,0.00048614905],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983406,0.000016297403,0.0000065800823,0.000050969888,0.00006337385,0.000028737302],"domain_scores_gemma":[0.99962103,0.000079504964,0.00008242693,0.0000797726,0.00008226312,0.000055003246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042736903,0.0002054278,0.0002452993,0.0013721988,0.00023922409,0.00084375637,0.00019236263,0.00021184514,0.0009838224],"category_scores_gemma":[0.0010139447,0.00015145875,0.0002479101,0.0006754478,0.0002490736,0.0006058196,0.00066624215,0.00024501834,0.00036970802],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007088033,0.000099323384,0.77882695,0.00016087557,0.00021248621,0.0015778698,0.0006433167,0.017778648,0.07279545,0.0028447332,0.0034978925,0.12085365],"study_design_scores_gemma":[0.000074591415,0.0001640555,0.6394123,0.00008977284,0.0001580265,0.0016602053,0.00055226934,0.28715974,0.045488454,0.004643868,0.020527504,0.00006925545],"about_ca_topic_score_codex":0.002439002,"about_ca_topic_score_gemma":0.0028936602,"teacher_disagreement_score":0.002439002,"about_ca_system_score_codex":0.00027241162,"about_ca_system_score_gemma":0.0002507642,"threshold_uncertainty_score":0.0048496723},"labels":[],"label_agreement":null},{"id":"W4226108066","doi":"10.3847/1538-4357/ac51c8","title":"Extreme Variation in Star Formation Efficiency across a Compact, Starburst Disk Galaxy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Astrophysics; Star formation; RADIUS; Galaxy; Metallicity; Velocity dispersion; Sigma; Spiral galaxy; Star (game theory); Effective radius; Inflow; Astronomy","score_opus":0.012605976061656267,"score_gpt":0.22821610245122956,"score_spread":0.2156101263895733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226108066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995813,0.000022775714,0.00006945296,0.000002587588,2.7320326e-7,5.2687074e-7,0.00009161333,0.000009125167,0.00022240425],"genre_scores_gemma":[0.9996711,0.0000088217075,0.000048641792,0.000002604083,6.103625e-7,9.16233e-7,0.00019297004,0.000003771139,0.000070700204],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982435,0.00002111127,0.00001043964,0.00006834497,0.000033702847,0.000042041433],"domain_scores_gemma":[0.99931395,0.00015799583,0.0001930704,0.00012664546,0.00008275923,0.00012550422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024198007,0.00014488104,0.0002329561,0.0008804355,0.0001414989,0.0005452899,0.00015371505,0.00017162439,0.0005726164],"category_scores_gemma":[0.0009228644,0.0001047917,0.00012734455,0.00050293223,0.00034068583,0.00019276528,0.0003614486,0.00014607566,0.0002667018],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012666127,0.000023245297,0.96961707,0.000007319593,0.000060333394,0.000083094856,0.00028647404,0.0006902208,0.024584472,0.000072060684,0.00013498616,0.0043140035],"study_design_scores_gemma":[0.0000011651866,0.000020156856,0.9983895,8.6512966e-7,0.000006789059,0.00006803698,0.000052995794,0.0004341599,0.0008873966,0.000014267121,0.00012208862,0.0000026131904],"about_ca_topic_score_codex":0.0020677103,"about_ca_topic_score_gemma":0.002120878,"teacher_disagreement_score":0.0020677103,"about_ca_system_score_codex":0.00026437241,"about_ca_system_score_gemma":0.000048593392,"threshold_uncertainty_score":0.00411129},"labels":[],"label_agreement":null},{"id":"W4226119674","doi":"10.3847/1538-4357/acc65b","title":"The Aemulus Project. V. Cosmological Constraint from Small-scale Clustering of BOSS Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":58,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"SLAC National Accelerator Laboratory; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Sigma; Planck; Correlation function (quantum field theory); Boss; Halo; Cosmology; Astronomy; Quantum mechanics","score_opus":0.018067471033187236,"score_gpt":0.23453437483665476,"score_spread":0.21646690380346753,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226119674","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6248693,0.0012286416,0.17121924,0.0018276024,0.00036226425,0.0002666509,0.054582138,0.07136992,0.07427423],"genre_scores_gemma":[0.8242972,0.0003255732,0.094268106,0.00039598587,0.00012983207,0.0003842143,0.060050085,0.008804295,0.011344699],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99941266,0.00027145972,0.000017842425,0.000082163424,0.00015073647,0.00006509854],"domain_scores_gemma":[0.99906677,0.00027796588,0.00012018998,0.00028069553,0.00013451143,0.000119998935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018737797,0.0005827792,0.0005030979,0.00080209045,0.00028276237,0.001028669,0.00089956005,0.0004172161,0.009081316],"category_scores_gemma":[0.0031112467,0.00027460806,0.0004308141,0.00068267365,0.0003359977,0.0008006404,0.00091234426,0.0003678835,0.0044395],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0035773546,0.00084856164,0.10772481,0.00081518723,0.0005313562,0.00047167088,0.00035841242,0.3386316,0.022710403,0.14494665,0.17705654,0.2023275],"study_design_scores_gemma":[0.00026319764,0.00013305417,0.020901915,0.00006812107,0.000040561354,0.0001364008,0.000039178787,0.8747154,0.014879245,0.027467158,0.061311778,0.000043950273],"about_ca_topic_score_codex":0.0037139922,"about_ca_topic_score_gemma":0.0028596746,"teacher_disagreement_score":0.009081316,"about_ca_system_score_codex":0.0006983914,"about_ca_system_score_gemma":0.0005058614,"threshold_uncertainty_score":0.03038001},"labels":[],"label_agreement":null},{"id":"W4226140351","doi":"10.3847/1538-4357/ac7d54","title":"The Dark Matter Halo of M54","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Dark matter halo; Astronomy; Dark matter; Dwarf galaxy; Halo; Galactic halo; Velocity dispersion; Dark galaxy; Galaxy","score_opus":0.00820541847331094,"score_gpt":0.2516271909525094,"score_spread":0.24342177247919847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226140351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983929,0.00003314076,0.000033466946,0.000020939844,0.0000013110526,0.0000013404177,0.00003979092,0.0000028405072,0.0014741524],"genre_scores_gemma":[0.99936527,0.000017983364,0.00006759115,0.000011411969,0.000001615126,0.0000013559593,0.00009783061,0.0000021369292,0.00043470302],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994147,0.000005882274,0.000002414748,0.000011602326,0.000009497326,0.000029077257],"domain_scores_gemma":[0.9998971,0.000008805283,0.000029318886,0.000014192973,0.000018145163,0.000032428143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008177673,0.0001721203,0.00012129123,0.00055334397,0.00053200254,0.0003831294,0.00017581631,0.00014345493,0.0028888572],"category_scores_gemma":[0.0003166856,0.00008958993,0.00013156414,0.00023736943,0.00043318924,0.00020042008,0.00075384515,0.00013518728,0.0006021943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042894037,0.000057912413,0.87884325,0.000031087984,0.00005547611,0.0021065015,0.0023411936,0.0004966915,0.090600185,0.005851025,0.0013127314,0.017875094],"study_design_scores_gemma":[0.000016950842,0.00012974265,0.9866698,0.000018423178,0.000020704945,0.0010499002,0.0011401417,0.000616915,0.0034506812,0.001214791,0.005658728,0.000013334108],"about_ca_topic_score_codex":0.011601309,"about_ca_topic_score_gemma":0.00578528,"teacher_disagreement_score":0.011601309,"about_ca_system_score_codex":0.0005762406,"about_ca_system_score_gemma":0.00012473755,"threshold_uncertainty_score":0.023067534},"labels":[],"label_agreement":null},{"id":"W4226152776","doi":"10.3847/1538-4357/ac650a","title":"The Eel Pulsar Wind Nebula: A PeVatron-candidate Origin for HAWC J1826−128 and HESS J1826−130","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Canadian Space Agency; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Physics; Pulsar wind nebula; Astrophysics; Pulsar; Cherenkov radiation; Nebula; Observatory; Astronomy; Stars","score_opus":0.013618946903586832,"score_gpt":0.2473773458988173,"score_spread":0.23375839899523046,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226152776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972343,0.00014591958,0.00016078963,0.00006841984,0.000013882793,0.0000095257565,0.00018773112,0.000014697622,0.00216473],"genre_scores_gemma":[0.9988858,0.000041736,0.00017356696,0.000033022312,0.000013917619,0.0000036564313,0.00040538673,0.00000620649,0.00043660082],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999434,0.0000025061465,0.0000020457107,0.000023792672,0.0000104823475,0.000017800356],"domain_scores_gemma":[0.99975187,0.000013757163,0.00006541686,0.000019290308,0.00002951593,0.00012006749],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012296608,0.00021565106,0.00023084895,0.00068973936,0.000639263,0.0007526611,0.00026777294,0.00025109077,0.0022827596],"category_scores_gemma":[0.00021281287,0.00010161404,0.00015671644,0.00039536558,0.0002844184,0.00021384351,0.0005065324,0.00029463504,0.0005296183],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002503067,0.00007238441,0.9433564,0.000029720448,0.000040777828,0.0029332612,0.0002733915,0.00019552966,0.04178148,0.00046416727,0.00077329646,0.009829327],"study_design_scores_gemma":[0.000015588015,0.000046035682,0.99394906,0.000011814014,0.000012731987,0.001081737,0.00032585542,0.00070524897,0.0013157234,0.0001425323,0.002387241,0.000006432566],"about_ca_topic_score_codex":0.0032371355,"about_ca_topic_score_gemma":0.004902362,"teacher_disagreement_score":0.0032371355,"about_ca_system_score_codex":0.0003470519,"about_ca_system_score_gemma":0.00016570729,"threshold_uncertainty_score":0.0076366067},"labels":[],"label_agreement":null},{"id":"W4226218711","doi":"10.3847/1538-4357/ac6187","title":"Evolution of a Peculiar Type Ibn Supernova SN 2019wep","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Astrophysics; Supernova; Physics; Light curve; Luminosity; Ejecta; Ion; Spectral line; Astronomy; Galaxy","score_opus":0.009811405596091283,"score_gpt":0.22328482104919561,"score_spread":0.21347341545310433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226218711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977053,0.000083538216,0.00019910505,0.000018133587,0.000013993934,0.000009918748,0.0009409861,0.000021127691,0.0010078045],"genre_scores_gemma":[0.9958515,0.00005776829,0.00030649817,0.000019344308,0.000012090245,0.000007696381,0.0030683246,0.000009150833,0.00066762243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998722,0.000008090877,0.000008293227,0.000048973525,0.000033373803,0.000028994142],"domain_scores_gemma":[0.9997205,0.000016215297,0.00007210755,0.00003076166,0.00006238847,0.00009810966],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021426333,0.00032484997,0.00030742053,0.0009119831,0.0004824313,0.0005823291,0.00021555918,0.00024530423,0.00065201503],"category_scores_gemma":[0.00026254577,0.00013720803,0.00029652228,0.00064879545,0.00018374392,0.00018840273,0.0005849596,0.00022865138,0.0003248212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004262202,0.00014569628,0.9247077,0.000044813612,0.00014317903,0.003506487,0.00019142067,0.0007782405,0.05528854,0.00023511755,0.0009437834,0.013588743],"study_design_scores_gemma":[0.0000022714835,0.00009754252,0.995275,0.0000046647924,0.000013807832,0.0009819095,0.00009143054,0.00052185036,0.0016938546,0.000038411607,0.0012733991,0.0000057356374],"about_ca_topic_score_codex":0.006748399,"about_ca_topic_score_gemma":0.010633652,"teacher_disagreement_score":0.006748399,"about_ca_system_score_codex":0.00036487886,"about_ca_system_score_gemma":0.00014300273,"threshold_uncertainty_score":0.013418257},"labels":[],"label_agreement":null},{"id":"W4226256235","doi":"10.3847/1538-4357/ac6ad0","title":"Narrowband Searches for Continuous and Long-duration Transient Gravitational Waves from Known Pulsars in the LIGO-Virgo Third Observing Run","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Polytechnique Montréal; Canadian Institute for Theoretical Astrophysics; University of Toronto; Université de Montréal; University of British Columbia","funders":"Astrophysics Division; Astrophysics Science Division; National Research, Development and Innovation Office; Institute for Cosmic Ray Research, University of Tokyo; Science and Engineering Research Board; Japan Society for the Promotion of Science; McGill Space Institute; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; Great Southern Development Commission, Government of Western Australia; Agencia Estatal de Investigación; Govern de les Illes Balears; Agencia Nacional de Investigación y Desarrollo; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; Canadian Institute for Advanced Research; National Astronomical Observatory of Japan; Ministry of Education, India; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Nuclear Safety and Security Commission; Hungarian Scientific Research Fund; University of Toronto; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; McGill University; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Smithsonian Institution; U.S. Department of Energy; Kavli Foundation; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Korea Institute of Science and Technology Information; Fondation familiale Trottier; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Culture, Sports, Science and Technology; European Regional Development Fund; ICTP South American Institute for Fundamental Research; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; Russian Science Foundation; University of British Columbia; Scottish Funding Council; Engineering and Physical Sciences Research Council; European Commission; Leverhulme Trust; European Social Fund; Royal Society; National Science Foundation; Fundacja na rzecz Nauki Polskiej; Compute Canada; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Australian Research Council; Western Canada Research Grid; Institut des Origines de Lyon; Centres de Recerca de Catalunya; National Aeronautics and Space Administration; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Ministerio de Ciencia e Innovación","keywords":"LIGO; Physics; Gravitational wave; Pulsar; Narrowband; Astrophysics; Transient (computer programming); Astronomy; Optics","score_opus":0.02115071011862567,"score_gpt":0.3017820465560121,"score_spread":0.2806313364373864,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226256235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99852777,0.0000331638,0.0005813103,0.00001814369,0.000001799284,0.000004551335,0.00027603854,0.000020650614,0.0005364444],"genre_scores_gemma":[0.99820554,0.000018596778,0.0006261541,0.000017282042,0.0000032325538,0.000007417434,0.001012981,0.0000110570045,0.00009770861],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958223,0.00006377059,0.00003116719,0.000089416375,0.000118306845,0.000114988004],"domain_scores_gemma":[0.997468,0.00050888496,0.001059567,0.00029970374,0.00012873573,0.00053502864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065646577,0.00023983775,0.00039446505,0.0011305365,0.00057429087,0.00078650075,0.00033060092,0.0003519967,0.00075011165],"category_scores_gemma":[0.0014120169,0.00015216094,0.00041115866,0.0012499582,0.00041281563,0.00028292768,0.0010770782,0.00037552288,0.00019580964],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010473067,0.00009850088,0.9444866,0.000035362384,0.00021118674,0.00030364725,0.0005472355,0.0007915112,0.03740863,0.0002775092,0.00036252404,0.014430047],"study_design_scores_gemma":[0.000023245593,0.00011114648,0.99382645,0.0000070700326,0.000052324787,0.00018464138,0.0002239229,0.0011828396,0.003599797,0.00016027683,0.0006175526,0.000010667197],"about_ca_topic_score_codex":0.0033048529,"about_ca_topic_score_gemma":0.010162293,"teacher_disagreement_score":0.0033048529,"about_ca_system_score_codex":0.0002780694,"about_ca_system_score_gemma":0.00042695896,"threshold_uncertainty_score":0.0065712333},"labels":[],"label_agreement":null},{"id":"W4226371544","doi":"10.3847/1538-4357/ad054a","title":"On the Formation and Interaction of Multiple Supermassive Stars in Cosmological Flows","year":2023,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Herzberg Institute of Astrophysics","funders":"National Research Council Canada; Universität Wien; Science and Technology Facilities Council; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; National Science Foundation","keywords":"Physics; Supermassive black hole; Astrophysics; Stars; Halo; Gamma-ray burst progenitors; Astronomy; Quasar; Accretion (finance); Redshift; Galaxy formation and evolution; Intermediate-mass black hole; Galaxy","score_opus":0.04163055002094625,"score_gpt":0.30057207323285157,"score_spread":0.25894152321190533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226371544","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965109,0.00012235463,0.0012520466,0.00022401144,0.000012041617,0.000014986878,0.00007170414,0.000028834978,0.0017631724],"genre_scores_gemma":[0.99859554,0.00006777634,0.00081053516,0.0000425744,0.000014020239,0.000008239928,0.00006211422,0.000010538235,0.00038855686],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986327,0.00004613672,0.0000055763303,0.000020272268,0.000018453464,0.000046170826],"domain_scores_gemma":[0.9988538,0.00028262567,0.00031747014,0.000050262697,0.00006548374,0.00043032347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007784283,0.00039158887,0.00055738713,0.0008813201,0.001266991,0.0011893077,0.00094307185,0.00096831215,0.0024263726],"category_scores_gemma":[0.0024677247,0.00040407258,0.0005265072,0.00043450517,0.00094845454,0.0008261607,0.0014925153,0.00053244137,0.00020016647],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005605338,0.00071937527,0.2993811,0.00012848292,0.0004937003,0.0022063649,0.0011465765,0.6138977,0.015210955,0.051506825,0.0032836308,0.011464766],"study_design_scores_gemma":[0.00014255855,0.00014031788,0.07754857,0.000024796884,0.000075700154,0.00016214844,0.00031514655,0.9090901,0.0010173613,0.009862466,0.001564022,0.00005681035],"about_ca_topic_score_codex":0.011349428,"about_ca_topic_score_gemma":0.006673156,"teacher_disagreement_score":0.011349428,"about_ca_system_score_codex":0.0013690556,"about_ca_system_score_gemma":0.0008015843,"threshold_uncertainty_score":0.022566736},"labels":[],"label_agreement":null},{"id":"W4226519477","doi":"10.3847/1538-4357/ac2430","title":"Competitive X-Ray and Optical Cooling in the Collisionless Shocks of WR 140","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"National Aeronautics and Space Administration","keywords":"Astrophysics; Physics; Luminosity; Stars; Context (archaeology); Absorption (acoustics); Plasma; Orbital period; Astronomy; Optics","score_opus":0.013326278398576715,"score_gpt":0.24312868839189555,"score_spread":0.22980240999331883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4226519477","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998574,0.0000086854225,0.000019089272,0.0000012710078,1.9409474e-7,4.609084e-7,0.000012313363,0.0000015998255,0.00009892608],"genre_scores_gemma":[0.99980897,0.0000062309523,0.000026554115,0.0000022059305,6.4371574e-7,6.6859616e-7,0.000073368064,0.0000014437462,0.00008001995],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993324,0.0000047871436,0.00000497581,0.000018682054,0.00001718254,0.000021157168],"domain_scores_gemma":[0.99986947,0.000012044375,0.000059388836,0.000010975902,0.000011710135,0.000036510533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011881459,0.00016449117,0.00022543762,0.00047099835,0.0002656367,0.00046248143,0.00018672325,0.0001767662,0.0005667344],"category_scores_gemma":[0.0003499902,0.0001348515,0.00014201578,0.00029452352,0.0001938644,0.00016409875,0.00048254424,0.00017524959,0.00014101857],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002562301,0.000045650268,0.93138826,0.000014800147,0.000039379647,0.0007098102,0.00034135007,0.000402776,0.06248386,0.00018737397,0.00005178994,0.004078819],"study_design_scores_gemma":[0.0000028687748,0.00006902725,0.9978259,0.0000011346067,0.0000062987765,0.00024798213,0.00012977947,0.00035998787,0.0011729654,0.000037949445,0.00014407591,0.0000019841123],"about_ca_topic_score_codex":0.0029079407,"about_ca_topic_score_gemma":0.0034897197,"teacher_disagreement_score":0.0029079407,"about_ca_system_score_codex":0.00026134003,"about_ca_system_score_gemma":0.00009591848,"threshold_uncertainty_score":0.005782008},"labels":[],"label_agreement":null},{"id":"W4229004881","doi":"10.3847/1538-4357/ac7c6c","title":"Young, Blue, and Isolated Stellar Systems in the Virgo Cluster. II. A New Class of Stellar System","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Agencia Nacional de Investigación y Desarrollo; Consejería de Economía, Conocimiento, Empresas y Universidad, Junta de Andalucía; Istituto Nazionale di Astrofisica; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Virgo Cluster; Ram pressure; Galaxy; Young stellar object; Cluster (spacecraft); Stars; Star formation; Galaxy cluster; Stellar mass; Astronomy","score_opus":0.009850480046682977,"score_gpt":0.23907829543688858,"score_spread":0.2292278153902056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229004881","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99621505,0.0009048215,0.00026481293,0.000111506415,0.000009919255,0.000009426159,0.000048298927,0.000012232978,0.0024237959],"genre_scores_gemma":[0.9987676,0.0001674571,0.00023777652,0.00006188378,0.000014350101,0.000005043397,0.00010430174,0.0000036370905,0.0006378939],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982375,0.000017569277,0.000006565835,0.000042443287,0.000038233018,0.00007145239],"domain_scores_gemma":[0.99967206,0.000038404807,0.000061839426,0.00002085239,0.000032480973,0.00017435051],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029170333,0.00020607421,0.00024250554,0.0015699181,0.0009308343,0.0011125024,0.0003475023,0.0004308566,0.0014667663],"category_scores_gemma":[0.00040627533,0.00010708947,0.00024464112,0.0005588604,0.0010863991,0.0004898865,0.0010360393,0.00031258064,0.00027813172],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004386641,0.0000937508,0.9574716,0.00005745231,0.00004259724,0.00082403485,0.0021139416,0.00087944715,0.008060461,0.0053124647,0.0008028627,0.023902593],"study_design_scores_gemma":[0.000052716612,0.00028253565,0.9821187,0.000040325824,0.000057386253,0.0016224263,0.0021062961,0.0021570702,0.00084899156,0.0049004713,0.0057866387,0.000026272643],"about_ca_topic_score_codex":0.005588767,"about_ca_topic_score_gemma":0.010065203,"teacher_disagreement_score":0.005588767,"about_ca_system_score_codex":0.0008997665,"about_ca_system_score_gemma":0.00033918617,"threshold_uncertainty_score":0.011112452},"labels":[],"label_agreement":null},{"id":"W4229010954","doi":"10.3847/1538-4357/ac6fd5","title":"The PAndAS View of the Andromeda Satellite System. III. Dwarf Galaxy Detection Limits","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Agence Nationale de la Recherche","keywords":"Andromeda; Dwarf galaxy; Astronomy; Satellite galaxy; Satellite; Andromeda Galaxy; Galaxy; Astrophysics; Physics; Spiral galaxy; Milky Way","score_opus":0.009918401203002143,"score_gpt":0.21022187202447656,"score_spread":0.20030347082147443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229010954","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.51046914,0.007280402,0.061131533,0.0037179939,0.00056368386,0.00020124219,0.080905475,0.027489921,0.3082406],"genre_scores_gemma":[0.9302424,0.0005719162,0.043127112,0.00031629577,0.00017281568,0.00006650982,0.0157757,0.000904026,0.0088232],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954766,0.00009501434,0.0000158174,0.00014260349,0.00013853144,0.00006028235],"domain_scores_gemma":[0.99930024,0.0001554742,0.00012818864,0.0001825873,0.00015153801,0.00008194971],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063270616,0.00037351315,0.00024089127,0.0016157835,0.0004441248,0.0012332017,0.00049988966,0.00036628058,0.0074135535],"category_scores_gemma":[0.001452405,0.00027764554,0.00025610946,0.0010012849,0.00031368522,0.0007900139,0.0007614691,0.00040350002,0.002943304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014043106,0.00012009689,0.40592417,0.0006692369,0.0003160621,0.00071817124,0.0009450497,0.010170732,0.044527855,0.03619788,0.11719684,0.3818095],"study_design_scores_gemma":[0.00009104652,0.0001275695,0.5769795,0.00019426795,0.00010467604,0.0019300034,0.0007011667,0.032418013,0.011317253,0.0105774505,0.365461,0.00009805825],"about_ca_topic_score_codex":0.011608704,"about_ca_topic_score_gemma":0.026951762,"teacher_disagreement_score":0.011608704,"about_ca_system_score_codex":0.00035802784,"about_ca_system_score_gemma":0.00027599942,"threshold_uncertainty_score":0.024800837},"labels":[],"label_agreement":null},{"id":"W4229016905","doi":"10.3847/1538-4357/ac680a","title":"Erratum: “Identification of Faint Chandra X-Ray Sources in the Core-collapsed Globular Cluster NGC 6397: Evidence for a Bimodal Cataclysmic Variable Population” (2010, ApJ, 722, 20)","year":2022,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; McGill University","funders":"","keywords":"Physics; Globular cluster; Astrophysics; Cataclysmic variable star; Population; Astronomy; Cluster (spacecraft); White dwarf; Galaxy; Stars; Medicine","score_opus":0.03116775571854359,"score_gpt":0.2715539985245445,"score_spread":0.2403862428060009,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229016905","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0027349808,0.0015771165,0.0011456874,0.03526781,0.9401108,0.000054490123,0.0051082694,0.00081503426,0.013185781],"genre_scores_gemma":[0.045657303,0.010563306,0.017596042,0.09832344,0.16108683,0.00022390303,0.025711183,0.0040097893,0.6368281],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99902916,0.00007510069,0.00023229847,0.00015207462,0.000445192,0.00006613514],"domain_scores_gemma":[0.9912145,0.0012789022,0.0006887009,0.0007199161,0.00568055,0.00041749355],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012879996,0.0018121041,0.0008409262,0.003198835,0.0025389197,0.0017719631,0.0018328286,0.0022869392,0.031114822],"category_scores_gemma":[0.014130655,0.00075802364,0.00079523417,0.0021594872,0.00093675393,0.0015692179,0.0009846565,0.0037478162,0.028816825],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036920854,0.000021304075,0.0005827719,0.00009232436,0.000011773702,0.0003574745,0.00003456875,0.000048612237,0.00020252222,0.00038889638,0.98876137,0.009461569],"study_design_scores_gemma":[0.000036544214,0.000048169037,0.009651285,0.00026460478,0.00006313991,0.0009777459,0.00017022609,0.00024322938,0.0010686121,0.00060331344,0.986822,0.000051143037],"about_ca_topic_score_codex":0.029228196,"about_ca_topic_score_gemma":0.036979668,"teacher_disagreement_score":0.031114822,"about_ca_system_score_codex":0.0018570201,"about_ca_system_score_gemma":0.0028847312,"threshold_uncertainty_score":0.10408944},"labels":[],"label_agreement":null},{"id":"W4229046764","doi":"10.3847/1538-4357/ac6424","title":"21cmVAE: A Very Accurate Emulator of the 21 cm Global Signal","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Reionization; Artificial neural network; SIGNAL (programming language); Code (set theory); Set (abstract data type); Computer science; COSMIC cancer database; Sky; Data set; Epoch (astronomy); Algorithm; Artificial intelligence; Physics; Astrophysics; Redshift; Computer vision; Stars","score_opus":0.009432759817904023,"score_gpt":0.22572391132364011,"score_spread":0.21629115150573608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229046764","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.28094518,0.00039171908,0.6215421,0.0005241793,0.0003719128,0.00018712018,0.010546225,0.07206578,0.013425701],"genre_scores_gemma":[0.724834,0.00013560613,0.24983701,0.00031075857,0.00007843798,0.0002544796,0.014932704,0.005465177,0.0041517443],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999819,0.00003306978,0.000010233155,0.00006154479,0.000054223237,0.000021997377],"domain_scores_gemma":[0.9995615,0.00016402554,0.000041797182,0.00009161177,0.00010436263,0.000036600508],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008890913,0.00071297033,0.00036326042,0.00079168536,0.00029824296,0.0007818003,0.0011612169,0.00068253244,0.006975786],"category_scores_gemma":[0.0032157414,0.00034133586,0.00050267775,0.00063222635,0.00023997636,0.0010357146,0.0008560275,0.0009699063,0.0019188859],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007363532,0.00023517046,0.022937981,0.0002151006,0.00038362984,0.00021996522,0.00023110137,0.74445623,0.02388751,0.012027008,0.035337478,0.15933244],"study_design_scores_gemma":[0.000040463543,0.00003851592,0.0032939056,0.000011299214,0.000011615188,0.00003369654,0.0000182296,0.9766025,0.011080813,0.0021381883,0.006707527,0.000023247894],"about_ca_topic_score_codex":0.00412493,"about_ca_topic_score_gemma":0.004085213,"teacher_disagreement_score":0.006975786,"about_ca_system_score_codex":0.00050891825,"about_ca_system_score_gemma":0.00057734974,"threshold_uncertainty_score":0.02333635},"labels":[],"label_agreement":null},{"id":"W4229452611","doi":"10.3847/1538-4357/ac8792","title":"Deep Two-phase, Hemispherical Magma Oceans on Lava Planets","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"McGill Space Institute; European Commission; Université de Paris; Agence Nationale de la Recherche; Labex UnivEarthS; Institut de Physique du Globe de Paris; McGill University","keywords":"Planet; Lava; Geology; Mantle (geology); Exoplanet; Magma; Astrobiology; Atmosphere (unit); Terrestrial planet; Geophysics; Volcano; Physics; Geochemistry; Astronomy; Meteorology","score_opus":0.009779869086058702,"score_gpt":0.24045335368768148,"score_spread":0.23067348460162276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229452611","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99854314,0.000036206,0.00028398976,0.000031750627,0.0000013271596,0.0000016493252,0.0002184407,0.000026950082,0.00085660047],"genre_scores_gemma":[0.9996991,0.00001157166,0.00005807417,0.000002882483,0.0000011962809,6.496429e-7,0.0001184617,0.0000031626078,0.00010496656],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994445,0.000007952821,0.0000028518239,0.000018550423,0.000010078709,0.000016063901],"domain_scores_gemma":[0.99975675,0.00005707523,0.00004666188,0.000037288835,0.00004271966,0.000059469872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013587727,0.00023717033,0.00020687093,0.0002935919,0.0003922743,0.0004896377,0.00035480573,0.00041775045,0.0011909067],"category_scores_gemma":[0.00062799343,0.00017440443,0.0003142186,0.00023692333,0.00029288378,0.0005213686,0.00055661675,0.00023422022,0.00017641917],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028273105,0.00009969265,0.79795897,0.00006095996,0.00015185722,0.00029560697,0.00025125427,0.07765273,0.11290701,0.002256403,0.00047714985,0.0076056453],"study_design_scores_gemma":[0.000031004412,0.00006227298,0.8649279,0.00000604169,0.000025921441,0.000060997907,0.0001239824,0.12027917,0.012560848,0.0010407782,0.00086361927,0.00001752354],"about_ca_topic_score_codex":0.015188264,"about_ca_topic_score_gemma":0.012042637,"teacher_disagreement_score":0.015188264,"about_ca_system_score_codex":0.0007126059,"about_ca_system_score_gemma":0.00020642739,"threshold_uncertainty_score":0.030199766},"labels":[],"label_agreement":null},{"id":"W4229454017","doi":"10.3847/1538-4357/ac6dd5","title":"Searching for Broadband Pulsed Beacons from 1883 Stars Using Neural Networks","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Space Science and Extraterrestrial Life","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Beacon; Stars; Broadband; Computer science; Telecommunications; Computer vision","score_opus":0.028968255559765156,"score_gpt":0.28144993123792644,"score_spread":0.25248167567816127,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229454017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915308,0.00022090168,0.0054746005,0.00011498906,0.000011413182,0.000009868434,0.00069115736,0.00024129618,0.0017049679],"genre_scores_gemma":[0.9921753,0.00006328235,0.0055325995,0.000038396563,0.000010983,0.0000052914156,0.0015089001,0.000030665527,0.0006345776],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998307,0.00001927028,0.000006740934,0.000054406468,0.000049743823,0.000039128692],"domain_scores_gemma":[0.99956363,0.00010947048,0.00011356671,0.000045478202,0.000084677136,0.00008307213],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030546245,0.00031485464,0.0002812468,0.0011573364,0.00032227547,0.0005065905,0.00038858826,0.000394513,0.0012160839],"category_scores_gemma":[0.0007437585,0.00019484713,0.0003173747,0.00094099453,0.00019577642,0.00039474192,0.0006000109,0.00036156212,0.00058618793],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007675819,0.00028331092,0.6575381,0.00019940581,0.00030355575,0.00046057135,0.00065839326,0.03881092,0.14507541,0.0011036558,0.005910118,0.148889],"study_design_scores_gemma":[0.00009114747,0.00038087566,0.6061272,0.00004981236,0.00015031907,0.0004309491,0.0008398505,0.35426375,0.023926558,0.002491926,0.011189346,0.00005831397],"about_ca_topic_score_codex":0.004424064,"about_ca_topic_score_gemma":0.010296549,"teacher_disagreement_score":0.004424064,"about_ca_system_score_codex":0.00032531982,"about_ca_system_score_gemma":0.00025484237,"threshold_uncertainty_score":0.008796632},"labels":[],"label_agreement":null},{"id":"W4229563127","doi":"10.1088/0004-637x/698/2/1943","title":"SPECTROSCOPIC CONFIRMATION OF A MASSIVE RED-SEQUENCE-SELECTED GALAXY CLUSTER AT<i>z</i>= 1.34 IN THE SpARCS-SOUTH CLUSTER SURVEY","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":167,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Waterloo; University of Toronto","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Redshift; Cluster (spacecraft); Galaxy; Astrophysics; Velocity dispersion; Galaxy cluster; Astronomy; Computer science","score_opus":0.014066728857008597,"score_gpt":0.23505044724523477,"score_spread":0.22098371838822617,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4229563127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980221,0.000051606814,0.00010376994,0.000027264268,0.000006024481,0.00001233262,0.00030247067,0.000019670068,0.0014547448],"genre_scores_gemma":[0.9981516,0.000052611224,0.00034959157,0.00003785583,0.000011533743,0.000005414848,0.00095206907,0.0000050953927,0.0004342134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979025,0.000012779115,0.000012688909,0.000052445914,0.00007626499,0.000055599594],"domain_scores_gemma":[0.9993431,0.000046500314,0.000120267716,0.000047286405,0.00014252578,0.0003003456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035865797,0.0002679614,0.00028594807,0.0011890653,0.0009357562,0.0004965684,0.0004730138,0.00023216406,0.0017983794],"category_scores_gemma":[0.0005383026,0.00015996561,0.00015063993,0.000622777,0.0004116899,0.00017264842,0.00056068646,0.00026468895,0.0004625899],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017166823,0.00007429283,0.9556947,0.00004159545,0.00006469156,0.0011049113,0.0007049602,0.00019193557,0.033629727,0.00035042482,0.0014487754,0.006522338],"study_design_scores_gemma":[0.0000075475673,0.00006269449,0.9960886,0.0000054574557,0.000021788745,0.0006714713,0.00018582282,0.00015973224,0.0016170425,0.000030026917,0.0011452035,0.0000046464547],"about_ca_topic_score_codex":0.026658073,"about_ca_topic_score_gemma":0.05454085,"teacher_disagreement_score":0.026658073,"about_ca_system_score_codex":0.00069621374,"about_ca_system_score_gemma":0.00051803404,"threshold_uncertainty_score":0.053005755},"labels":[],"label_agreement":null},{"id":"W4231024935","doi":"10.1086/375508","title":"The Anisotropy of the Microwave Background to<i>l</i>= 3500: Mosaic Observations with the Cosmic Background Imager","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":281,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Cosmic microwave background; Astrophysics; Spectral density; Cosmic background radiation; Galaxy; Quasar; Reionization; Point source; Spectral line; Astronomy; Anisotropy; Optics; Redshift","score_opus":0.01650347520703211,"score_gpt":0.2265307503845573,"score_spread":0.2100272751775252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4231024935","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98861516,0.00018275481,0.0009779684,0.00014486078,0.000012410792,0.0000054237566,0.00088747765,0.00017783075,0.008996078],"genre_scores_gemma":[0.99765635,0.00005461853,0.0008650099,0.000030136101,0.000017167202,0.000002833541,0.00079231645,0.000044038366,0.0005375209],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999052,0.000011348094,0.0000023406283,0.000026080274,0.000027957405,0.000026958649],"domain_scores_gemma":[0.99983263,0.0000152067,0.00004210397,0.000022865219,0.00003441109,0.00005273517],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001874525,0.00010082759,0.00009283566,0.000531323,0.00020323852,0.0005182025,0.00015404093,0.00016674226,0.00082373613],"category_scores_gemma":[0.0004889295,0.00012483537,0.000100109435,0.00051601545,0.00016937844,0.0003095743,0.00038020805,0.00031284,0.00025102159],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014080008,0.00024580795,0.5519496,0.00009029816,0.00016915091,0.0005766352,0.0013474053,0.0027577968,0.33901572,0.0053089983,0.010343745,0.086786844],"study_design_scores_gemma":[0.000021829032,0.000024157785,0.989146,0.000007931106,0.00003393017,0.00013452035,0.0001192264,0.0022842095,0.003994179,0.00037799482,0.0038448563,0.0000111691315],"about_ca_topic_score_codex":0.0122543005,"about_ca_topic_score_gemma":0.026704747,"teacher_disagreement_score":0.0122543005,"about_ca_system_score_codex":0.00028875287,"about_ca_system_score_gemma":0.00021398689,"threshold_uncertainty_score":0.024365962},"labels":[],"label_agreement":null},{"id":"W4232310751","doi":"10.1088/0004-637x/693/1/186","title":"ON THE DYNAMICAL EVOLUTION OF H II REGIONS: AN INVESTIGATION OF THE IONIZED COMPONENT OF W4, A GALACTIC CHIMNEY CANDIDATE. II. KINEMATICS AND DYNAMICS IN THE LATITUDE RANGE 3° &lt;<i>b</i>⩽ 7°","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Redshift; Chimney (locomotive); Sky; Galactic Center; Astronomy; Galaxy; Meteorology","score_opus":0.010842520534741893,"score_gpt":0.22187457361230312,"score_spread":0.21103205307756123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4232310751","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993144,0.000032013555,0.00014466768,0.0000074149034,7.4570517e-7,0.000002887318,0.00003139154,0.000004941106,0.000461518],"genre_scores_gemma":[0.99850297,0.00006389734,0.00060386956,0.000011044974,0.0000049805158,0.0000044677763,0.00028916175,0.0000068505606,0.0005126825],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999966,0.000003692135,0.0000012756818,0.0000085249885,0.000006947198,0.000013529092],"domain_scores_gemma":[0.9998586,0.00001917088,0.000048989958,0.000010533226,0.00001961149,0.000042997715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010795575,0.0002417073,0.00013747886,0.0007887392,0.00040597763,0.00030107668,0.00038568873,0.00022499613,0.00092215213],"category_scores_gemma":[0.00017070977,0.000118931915,0.00016189352,0.00032971016,0.00027137523,0.0002434412,0.0005511464,0.00016573256,0.00035838952],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039557644,0.00011183603,0.76157045,0.000032068365,0.000048803013,0.001700268,0.0005267527,0.0007654086,0.22389157,0.00025366896,0.00021810274,0.010485494],"study_design_scores_gemma":[0.0000058686255,0.00016280338,0.9883825,0.0000029356718,0.000018269986,0.00043672774,0.00042070413,0.0016381807,0.007996004,0.00009761242,0.0008311104,0.0000072040634],"about_ca_topic_score_codex":0.0036556358,"about_ca_topic_score_gemma":0.006077427,"teacher_disagreement_score":0.0036556358,"about_ca_system_score_codex":0.00022665922,"about_ca_system_score_gemma":0.000104635335,"threshold_uncertainty_score":0.007268727},"labels":[],"label_agreement":null},{"id":"W4232393710","doi":"10.3847/1538-4357/abe627","title":"A Machine-learning Approach to Integral Field Unit Spectroscopy Observations. II. H ii Region Line Ratios","year":2021,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Chemometric Analyses","field":"Chemistry","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; Institut de Valorisation des Données; Université de Montréal; Mitacs; Institut national des sciences de l'Univers; Fundação de Amparo à Pesquisa e Inovação do Estado de Santa Catarina; Centre National de la Recherche Scientifique; Conselho Nacional de Desenvolvimento Científico e Tecnológico","keywords":"Artificial neural network; Algorithm; Computer science; Artificial intelligence; Line (geometry); Spectral line; Residual; Noise (video); Machine learning; Mathematics; Physics; Geometry","score_opus":0.036496903909694886,"score_gpt":0.27825992618858386,"score_spread":0.24176302227888896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4232393710","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47711504,0.00050158764,0.51781225,0.0003948946,0.000025750385,0.00005258301,0.00021142265,0.00058907707,0.0032973615],"genre_scores_gemma":[0.9313912,0.00007210367,0.06761178,0.00003132792,0.000022752585,0.00002125198,0.00014618083,0.000030305418,0.00067317736],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99978346,0.000083544895,0.000008036653,0.00007050822,0.00003822018,0.000016277645],"domain_scores_gemma":[0.999522,0.00022728094,0.00009192881,0.00006374163,0.000077483026,0.000017626295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074453076,0.00038217747,0.00020092273,0.000804762,0.00030331474,0.0004973348,0.0007383673,0.00049160654,0.0006392429],"category_scores_gemma":[0.0028163171,0.00019803194,0.00032734047,0.00068876654,0.0002933913,0.0006643672,0.00037594305,0.00056958915,0.00015487468],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009602353,0.000106052736,0.016742054,0.000046699686,0.00007130842,0.000057548794,0.00006112207,0.82656777,0.013327644,0.003942954,0.0005610628,0.13841978],"study_design_scores_gemma":[0.000001287934,0.0000074140435,0.0019759568,0.0000014115675,0.0000020973666,0.000007023674,0.000006141173,0.9954587,0.0012524852,0.0011676227,0.00011715158,0.0000027886417],"about_ca_topic_score_codex":0.0064490307,"about_ca_topic_score_gemma":0.0068852575,"teacher_disagreement_score":0.0064490307,"about_ca_system_score_codex":0.0007602235,"about_ca_system_score_gemma":0.00024829424,"threshold_uncertainty_score":0.012822986},"labels":[],"label_agreement":null},{"id":"W4235166508","doi":"10.3847/1538-4357/833/1/44","title":"THE JCMT GOULD BELT SURVEY: DENSE CORE CLUSTERS IN ORION A","year":2016,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Astrophysics; Molecular cloud; Star formation; Physics; Orion Nebula; Core (optical fiber); High mass; James Clerk Maxwell Telescope; Astronomy; Stars","score_opus":0.021165353631481507,"score_gpt":0.25991971629130534,"score_spread":0.23875436265982383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4235166508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99871397,0.00007731157,0.00005551432,0.000021607291,0.0000011466459,0.000008045146,0.0006169587,0.000011074987,0.0004944312],"genre_scores_gemma":[0.9979547,0.000058548838,0.0004347397,0.00001900451,0.0000069641046,0.000008062917,0.0012326131,0.000006438644,0.0002788921],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998648,0.000010964145,0.0000074395766,0.000039641982,0.000041093415,0.0000360091],"domain_scores_gemma":[0.9995048,0.000041319392,0.00018731726,0.000057341844,0.000052520314,0.00015662065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018137779,0.00012119145,0.00015002312,0.002257307,0.0004540291,0.0004167197,0.00028397134,0.00018446417,0.00075497705],"category_scores_gemma":[0.0007411912,0.00007538496,0.00011398177,0.0015948457,0.00025929642,0.00023111762,0.0008047827,0.00009769369,0.00014141257],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000070421374,0.000030681873,0.98142034,0.00002015041,0.00003065134,0.00018105026,0.0006612837,0.00013692598,0.010137005,0.00016444098,0.0006530334,0.006494027],"study_design_scores_gemma":[0.0000014520243,0.0000019305392,0.99948597,0.0000014700331,0.000002295182,0.00002350629,0.000053552416,0.000069890106,0.00009077451,0.000009587685,0.00025883704,7.8969293e-7],"about_ca_topic_score_codex":0.05835984,"about_ca_topic_score_gemma":0.100732036,"teacher_disagreement_score":0.05835984,"about_ca_system_score_codex":0.00044724063,"about_ca_system_score_gemma":0.00031168316,"threshold_uncertainty_score":0.11604029},"labels":[],"label_agreement":null},{"id":"W4238990203","doi":"10.1086/312493","title":"Submillimeter Polarimetry of the Protostellar Outflow Sources in Serpens with the Submillimeter Common-User Bolometer Array","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Serpens; Physics; Astrophysics; Submillimeter Array; Protostar; Astronomy; Polarization (electrochemistry); Outflow; Polarimetry; Intracluster medium; Molecular cloud; Star formation; Stars; Galaxy cluster; Galaxy; Optics","score_opus":0.005982213592743499,"score_gpt":0.20716479371187438,"score_spread":0.20118258011913087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4238990203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997024,0.00007992493,0.00033771512,0.000014908514,0.0000063206257,0.0000045285515,0.00053994317,0.000041531785,0.0019512626],"genre_scores_gemma":[0.9978517,0.000091886766,0.00074070843,0.000015312447,0.000015175588,0.0000034986467,0.00091204885,0.000009890362,0.00035968382],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994886,0.000005941573,0.0000031733691,0.000013732553,0.000013912647,0.000014288369],"domain_scores_gemma":[0.9998288,0.000025995123,0.00006827387,0.000019038727,0.000018869538,0.000039051523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011713415,0.0002356228,0.00013160543,0.0009590444,0.00019782246,0.000274684,0.0001275644,0.000107417254,0.00078064564],"category_scores_gemma":[0.0001982655,0.00012389944,0.00012727948,0.00050715654,0.00014177832,0.00012976848,0.00030494397,0.00016473839,0.00024690002],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037459342,0.00006527952,0.87485397,0.000047918926,0.00007832018,0.0005930239,0.00047061764,0.0013991902,0.081605345,0.00040623048,0.0008990902,0.039206415],"study_design_scores_gemma":[0.000005474536,0.000024937328,0.99630016,0.000005140497,0.000008984992,0.00014292722,0.0000723488,0.0004691666,0.001879078,0.000055367735,0.0010344045,0.0000021617102],"about_ca_topic_score_codex":0.003335182,"about_ca_topic_score_gemma":0.009555829,"teacher_disagreement_score":0.003335182,"about_ca_system_score_codex":0.000192561,"about_ca_system_score_gemma":0.0000994658,"threshold_uncertainty_score":0.006631553},"labels":[],"label_agreement":null},{"id":"W4244907507","doi":"10.1088/0004-637x/706/2/1504","title":"DISPERSION OF MAGNETIC FIELDS IN MOLECULAR CLOUDS. II.","year":2009,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":230,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Turbulence; Magnetic field; Physics; Polarization (electrochemistry); Molecular cloud; Computational physics; Dispersion (optics); Spatial correlation; Optics; Astrophysics; Meteorology; Statistics; Chemistry","score_opus":0.004923661776280817,"score_gpt":0.2198375094574082,"score_spread":0.2149138476811274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4244907507","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96183443,0.0018827877,0.027780943,0.00037824048,0.00006774865,0.000026759806,0.0004483705,0.0001814065,0.007399303],"genre_scores_gemma":[0.99665254,0.00032324472,0.0023919975,0.000029393015,0.000054134725,0.000005567852,0.00013381426,0.000016406535,0.000392875],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998776,0.0000099253675,0.0000065697463,0.000032218115,0.000044491324,0.000029222676],"domain_scores_gemma":[0.99951184,0.00012851976,0.00018827638,0.00007493554,0.000063371015,0.00003311036],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002941405,0.00014854415,0.00012835642,0.00095436064,0.00038872,0.0007177045,0.00024557428,0.00019606035,0.00064846437],"category_scores_gemma":[0.0017074569,0.00012563594,0.000123705,0.0006340185,0.0003849585,0.0004278402,0.0004967019,0.00036782722,0.00024085291],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002037257,0.000089990455,0.62011135,0.00019193604,0.000110263856,0.00049934105,0.00080121914,0.08527271,0.13276246,0.051872045,0.0019852172,0.10609981],"study_design_scores_gemma":[0.00005203617,0.00013997608,0.62962586,0.00008132607,0.00006012401,0.0011062217,0.000354874,0.2708185,0.04862985,0.036389466,0.012648947,0.00009277495],"about_ca_topic_score_codex":0.0043223933,"about_ca_topic_score_gemma":0.0029886542,"teacher_disagreement_score":0.0043223933,"about_ca_system_score_codex":0.00052974274,"about_ca_system_score_gemma":0.00018092748,"threshold_uncertainty_score":0.008594453},"labels":[],"label_agreement":null},{"id":"W4246376382","doi":"10.1088/0004-637x/795/1/29","title":"RADIO TIMING AND OPTICAL PHOTOMETRY OF THE BLACK WIDOW SYSTEM PSR J1518+0204C IN THE GLOBULAR CLUSTER M5","year":2014,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Universities Space Research Association; National Radio Astronomy Observatory; Space Telescope Science Institute; National Science Foundation","keywords":"Globular cluster; Photometry (optics); Physics; Astronomy; Astrophysics; Galaxy; Stars","score_opus":0.00855656688307667,"score_gpt":0.21350260671583698,"score_spread":0.2049460398327603,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4246376382","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994691,0.000030703697,0.000059291844,0.000005506392,0.0000016815567,0.0000026489465,0.00015178435,0.000008172405,0.00027110844],"genre_scores_gemma":[0.99872583,0.000028896784,0.00039784532,0.000009409358,0.0000053800004,0.0000039801853,0.0006411759,0.0000033246558,0.00018422883],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999112,0.0000059706185,0.0000056783706,0.000027840637,0.000023016491,0.000026306223],"domain_scores_gemma":[0.9997831,0.00001290176,0.00007619327,0.000018518196,0.000038253966,0.000071134295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016229956,0.00019073805,0.00015953011,0.0011256803,0.00030174223,0.00028988515,0.0003070766,0.00020898708,0.00071839325],"category_scores_gemma":[0.00036275742,0.000108334716,0.00010787805,0.0006270808,0.00016786662,0.00014381885,0.0003245602,0.00010774625,0.00022047242],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025523597,0.00006865888,0.935491,0.0000287746,0.000031046842,0.0004433985,0.00042028553,0.00035856088,0.050449673,0.00013458906,0.00036751205,0.011951118],"study_design_scores_gemma":[0.00000544479,0.00007845341,0.9975809,0.000003435054,0.000009277627,0.00016768872,0.00005983415,0.0004191015,0.0011286242,0.000014873032,0.00052913977,0.0000032421049],"about_ca_topic_score_codex":0.009590156,"about_ca_topic_score_gemma":0.014906539,"teacher_disagreement_score":0.009590156,"about_ca_system_score_codex":0.00034732147,"about_ca_system_score_gemma":0.00015882177,"threshold_uncertainty_score":0.019068658},"labels":[],"label_agreement":null},{"id":"W4248992227","doi":"10.3847/1538-4357/abefd2","title":"Erratum: “Simultaneous X-Ray and Infrared Observations of Sagittarius A*'s Variability” (2019, ApJ, 871, 161)","year":2021,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; McGill University","funders":"","keywords":"Physics; Sagittarius; Astrophysics; Infrared; Astronomy; X-ray; Optics; Stars; Milky Way","score_opus":0.012953665602539736,"score_gpt":0.22620051134951624,"score_spread":0.2132468457469765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4248992227","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0007588675,0.0011251745,0.00024575822,0.037240185,0.94183207,0.000026404794,0.0028281969,0.0003595159,0.015583837],"genre_scores_gemma":[0.015728258,0.0046260874,0.0025730517,0.08561524,0.1890836,0.00011593809,0.011957701,0.0011586852,0.6891415],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9991929,0.00007309664,0.00014515738,0.0001332757,0.0003590111,0.000096520154],"domain_scores_gemma":[0.9957287,0.0006418052,0.00029375363,0.00032826513,0.0025863945,0.0004211251],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010467282,0.001894072,0.0011178491,0.0029870535,0.004261886,0.003285337,0.0018177036,0.0037480155,0.05402089],"category_scores_gemma":[0.0076842722,0.00069912756,0.0010838412,0.0016213205,0.0010219354,0.0018699764,0.0014466178,0.004449482,0.041774873],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004353464,0.000009433397,0.000114896444,0.000037432983,0.0000057301904,0.00012328282,0.000010099972,0.000019539539,0.00011181532,0.00024307414,0.99692494,0.0023562463],"study_design_scores_gemma":[0.000032002903,0.000035611505,0.0047257417,0.0001280358,0.00003289859,0.00020946737,0.00010783804,0.00013387372,0.00047989763,0.0008579599,0.9932243,0.000032366068],"about_ca_topic_score_codex":0.03300843,"about_ca_topic_score_gemma":0.051496644,"teacher_disagreement_score":0.05402089,"about_ca_system_score_codex":0.0024366085,"about_ca_system_score_gemma":0.002965863,"threshold_uncertainty_score":0.18071783},"labels":[],"label_agreement":null},{"id":"W4280538156","doi":"10.3847/1538-4357/ac5624","title":"Sparse Identification of Variable Star Dynamics","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Tamkeen; Japan Society for the Promotion of Science; European Commission; New York University Abu Dhabi","keywords":"Algorithm; Physics; Computer science","score_opus":0.009054900704149906,"score_gpt":0.21273086593496457,"score_spread":0.20367596523081466,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280538156","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.53875923,0.0001276974,0.45633703,0.00028871946,0.00003202455,0.000048684342,0.0007451031,0.0013570442,0.0023044916],"genre_scores_gemma":[0.96300936,0.000040080846,0.03449787,0.00003328807,0.000015609186,0.00002570635,0.0011390161,0.000061147475,0.0011778075],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997216,0.000084727035,0.000017477609,0.000077823046,0.000056361896,0.000041915173],"domain_scores_gemma":[0.99792826,0.0009917555,0.00029799502,0.00038948067,0.00025965032,0.00013276903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00092344667,0.00042865056,0.0005286086,0.00075211155,0.00031319662,0.0007051095,0.00065951433,0.000504911,0.0017847483],"category_scores_gemma":[0.005301638,0.0003246955,0.0005939241,0.0003092973,0.0004016378,0.0009390541,0.001201426,0.0007803856,0.00053774443],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021611452,0.000102472324,0.05784737,0.00010397709,0.00010024404,0.00017288009,0.00025061308,0.8270337,0.006984504,0.010211411,0.0021084961,0.09486821],"study_design_scores_gemma":[0.0000024186752,0.000006109962,0.0014457923,0.000002170598,0.0000013369288,0.0000103727,0.0000091823085,0.99529475,0.00045603557,0.0026167023,0.00015209695,0.0000030838328],"about_ca_topic_score_codex":0.005037734,"about_ca_topic_score_gemma":0.004143565,"teacher_disagreement_score":0.005037734,"about_ca_system_score_codex":0.000474035,"about_ca_system_score_gemma":0.0006335244,"threshold_uncertainty_score":0.010016799},"labels":[],"label_agreement":null},{"id":"W4280575519","doi":"10.3847/1538-4357/ac8ff6","title":"The Diverse Properties of Type Icn Supernovae Point to Multiple Progenitor Channels","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"National Science Foundation","keywords":"Physics; Supernova; Astrophysics; Type (biology); Point (geometry); Progenitor; Astronomy; Progenitor cell; Genetics","score_opus":0.020920126191529047,"score_gpt":0.2238665527098793,"score_spread":0.20294642651835024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280575519","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971771,0.00022426555,0.000539537,0.0000062966865,0.0000034126888,0.000009003963,0.00032235406,0.000016003412,0.0017018866],"genre_scores_gemma":[0.99849415,0.00011925703,0.0003554413,0.0000070420483,0.000005243472,0.000004582536,0.00072766235,0.0000059308477,0.00028080985],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978226,0.00001939351,0.000020702406,0.000071146846,0.00006402475,0.000042523854],"domain_scores_gemma":[0.99947315,0.000113198534,0.00013182616,0.00008872066,0.00008747939,0.000105744024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003879359,0.000294938,0.00032246293,0.00111145,0.00039683573,0.0009418987,0.00032199753,0.00018546486,0.00115023],"category_scores_gemma":[0.00090083154,0.00012594373,0.00026572566,0.0010292561,0.00025865,0.0002495516,0.0004585312,0.00012495182,0.00029581436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014379037,0.000023021184,0.98189974,0.00002402316,0.00003815476,0.000337943,0.000058362115,0.00055214996,0.008131237,0.00036167464,0.00012639152,0.00830339],"study_design_scores_gemma":[0.0000057596044,0.00006533247,0.99102473,0.00001167165,0.00004665046,0.0018329052,0.00018072364,0.0015591903,0.0034699996,0.00039261996,0.0014036234,0.000006699659],"about_ca_topic_score_codex":0.0022646452,"about_ca_topic_score_gemma":0.0042246752,"teacher_disagreement_score":0.0022646452,"about_ca_system_score_codex":0.00027573906,"about_ca_system_score_gemma":0.0002045904,"threshold_uncertainty_score":0.0045028925},"labels":[],"label_agreement":null},{"id":"W4280576516","doi":"10.3847/1538-4357/ac6fce","title":"Modeling the Optical to Ultraviolet Polarimetric Variability from Thomson Scattering in Colliding-wind Binaries","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council","keywords":"Physics; Thomson scattering; Opacity; Polarization (electrochemistry); Scattering; Astrophysics; Wavelength; Polarimetry; Luminous blue variable; Stars; Optics","score_opus":0.02021804869652668,"score_gpt":0.2519018892341171,"score_spread":0.23168384053759042,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280576516","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9826822,0.00008798102,0.014556602,0.00008784921,0.000011174496,0.000019600631,0.00023279934,0.00010630434,0.002215463],"genre_scores_gemma":[0.9987117,0.00003345328,0.0008130048,0.000014768214,0.00000753324,0.0000074631125,0.00009343987,0.000016647049,0.00030193297],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999181,0.000015856269,0.0000038374733,0.000022905851,0.000016840242,0.000022500353],"domain_scores_gemma":[0.999721,0.00010777608,0.00007233094,0.000027016038,0.000029475976,0.000042472493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002739773,0.00039130193,0.00022743706,0.0004485492,0.0004048416,0.0009242072,0.0006132892,0.0006179803,0.00060641463],"category_scores_gemma":[0.00088466913,0.00027672085,0.00043874598,0.0005844725,0.0004120305,0.000597242,0.0005094162,0.0004813743,0.000124397],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007119403,0.000050959818,0.058474336,0.000013756191,0.00004409145,0.00018163655,0.000063790656,0.93145984,0.004178589,0.0020577086,0.0002569972,0.0031471667],"study_design_scores_gemma":[0.000006552211,0.000007627448,0.012183603,0.0000018551589,0.0000065167587,0.000016762657,0.000013789822,0.9866753,0.00033365804,0.00064917706,0.000098104916,0.0000069734424],"about_ca_topic_score_codex":0.024390033,"about_ca_topic_score_gemma":0.009569965,"teacher_disagreement_score":0.024390033,"about_ca_system_score_codex":0.0009705801,"about_ca_system_score_gemma":0.0003422838,"threshold_uncertainty_score":0.048496127},"labels":[],"label_agreement":null},{"id":"W4280587093","doi":"10.3847/1538-4357/ac6e69","title":"Groups and Protocluster Candidates in the CLAUDS and HSC-SSP Joint Deep Surveys","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Saint Mary's University","funders":"National Key Research and Development Program of China; Higher Education Discipline Innovation Project; Overseas Expertise Introduction Project for Discipline Innovation; National Natural Science Foundation of China; Natural Science Foundation of Shanghai; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Redshift; Astrophysics; Galaxy; Halo; Photometric redshift; Sky; Astronomy; Galaxy cluster; Galaxy formation and evolution","score_opus":0.008451564593577477,"score_gpt":0.207818979503058,"score_spread":0.1993674149094805,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280587093","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949077,0.000090904796,0.00044782262,0.00001997298,0.000002893404,0.000007765757,0.0032313936,0.00006786284,0.00122377],"genre_scores_gemma":[0.9887262,0.000042335203,0.0008860918,0.000014680075,0.0000051796987,0.000006566738,0.009635021,0.000013514404,0.00067046395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968326,0.00003265608,0.000014583074,0.000076202894,0.000105926345,0.00008745932],"domain_scores_gemma":[0.9987684,0.00012297508,0.00035287812,0.0002001288,0.00020108363,0.0003545195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041900293,0.00015683423,0.00023606312,0.0037461696,0.00036254237,0.00057506096,0.00032693098,0.00015699283,0.0021773227],"category_scores_gemma":[0.0012787203,0.000101783946,0.00020591512,0.0022074927,0.00024343307,0.00029260942,0.0014608017,0.00014771869,0.00048158225],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012811321,0.000019041312,0.9800167,0.000018086641,0.000040693078,0.000070310605,0.00020454694,0.00070249644,0.002437223,0.00034035268,0.0020071387,0.014015269],"study_design_scores_gemma":[0.0000098969795,0.000019513387,0.9933856,0.0000075399244,0.000021180389,0.00006477245,0.00021627478,0.0023845355,0.0007698806,0.00017221777,0.0029413747,0.000007190277],"about_ca_topic_score_codex":0.013972387,"about_ca_topic_score_gemma":0.027293038,"teacher_disagreement_score":0.013972387,"about_ca_system_score_codex":0.00028054725,"about_ca_system_score_gemma":0.00033674005,"threshold_uncertainty_score":0.027782142},"labels":[],"label_agreement":null},{"id":"W4280641136","doi":"10.3847/1538-4357/ac6ce1","title":"A Multiwavelength Study of GRS 1716-249 in Outburst: Constraints on Its System Parameters","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Southern Observatory; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Japan Aerospace Exploration Agency; European Commission; New York University Abu Dhabi; Academy of Finland; National Natural Science Foundation of China; Isaac Newton Trust; University of Leicester; Leverhulme Trust; Ministerio de Ciencia, Innovación y Universidades; RIKEN; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Telescope; Observatory; Infrared; Light curve; Astronomy; Black hole (networking); Ultraviolet; Accretion (finance); Wavelength; Flux (metallurgy); Accretion disc; Optics","score_opus":0.029845043107186338,"score_gpt":0.2529530316917627,"score_spread":0.22310798858457637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280641136","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989415,0.00011233134,0.00010648165,0.000016701215,0.000004552996,0.000004419729,0.00024116432,0.00000993367,0.00056303525],"genre_scores_gemma":[0.99908316,0.000058286885,0.000118860466,0.00001129457,0.000008792882,0.0000033943993,0.00052064616,0.0000073756573,0.0001882021],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999039,0.000009164102,0.0000066438397,0.000026127318,0.000022202532,0.00003191745],"domain_scores_gemma":[0.9995252,0.000055650406,0.00020206487,0.000033608558,0.000054222455,0.00012930164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030977506,0.00029510114,0.00046012277,0.0010469292,0.00054373266,0.0007036582,0.0002854847,0.00024496764,0.00103507],"category_scores_gemma":[0.00044350163,0.00015479024,0.00026443065,0.00082691887,0.00028948966,0.0003504269,0.00055828143,0.00038411134,0.00031482492],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026708952,0.00008288547,0.96140414,0.000039547896,0.000048417725,0.00079590623,0.00046862217,0.00080802024,0.028370116,0.00019146477,0.00037433542,0.007149445],"study_design_scores_gemma":[0.0000025920756,0.000038601396,0.99819237,0.0000049083983,0.000008881894,0.00014075263,0.00019475259,0.00042313605,0.0005747874,0.000037543177,0.0003767425,0.000004859266],"about_ca_topic_score_codex":0.0064992676,"about_ca_topic_score_gemma":0.010922703,"teacher_disagreement_score":0.0064992676,"about_ca_system_score_codex":0.00046939086,"about_ca_system_score_gemma":0.00019364401,"threshold_uncertainty_score":0.012922883},"labels":[],"label_agreement":null},{"id":"W4280648416","doi":"10.3847/1538-4357/ac63ba","title":"Disk Evolution Study through Imaging of Nearby Young Stars (DESTINYS): A Panchromatic View of DO Tau’s Complex Kilo-astronomical-unit Environment","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"H2020 European Research Council; Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Fondo Nacional de Desarrollo Científico, Tecnológico y de Innovación Tecnológica; National Institutes of Natural Sciences; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; Deutsche Forschungsgemeinschaft; York University; Agence Nationale de la Recherche; European Southern Observatory; National Science Council; Space Telescope Science Institute; Eidgenössische Technische Hochschule Zürich; Carnegie Mellon University; College of Engineering, Michigan State University; Goddard Space Flight Center; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; U.S. Department of Energy; National Radio Astronomy Observatory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Harvard University; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Ohio State University; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Office National d'études et de Recherches Aérospatiales; National Science Foundation; European Commission; California Institute of Technology; National Aeronautics and Space Administration","keywords":"Physics; Panchromatic film; Stars; Astronomy; Astrophysics; Unit (ring theory); Image resolution; Optics","score_opus":0.01734578910479229,"score_gpt":0.24639918736600416,"score_spread":0.22905339826121188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4280648416","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975182,0.00009059104,0.0004465648,0.000028451825,0.000004827904,0.00000972238,0.00030404786,0.000024672789,0.0015730306],"genre_scores_gemma":[0.99768674,0.000059122696,0.0013265552,0.000018270732,0.000011846571,0.0000042004285,0.00036738138,0.000010212579,0.0005156228],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996746,0.0000020328657,0.0000017268774,0.000012375727,0.000006334173,0.000010131811],"domain_scores_gemma":[0.9998987,0.0000070538977,0.000019698033,0.0000092624605,0.000018650753,0.000046696463],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009036308,0.00016013607,0.0001080775,0.0008625264,0.00031232001,0.00032479886,0.00010242528,0.00015434615,0.0010400064],"category_scores_gemma":[0.00007861109,0.000108314984,0.00012297218,0.0003535038,0.00008848592,0.00022893216,0.00025333528,0.00012707138,0.00022434663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030035817,0.00011424298,0.6393849,0.00006382814,0.00005723597,0.00245424,0.0010723566,0.00034785547,0.33278725,0.00018796114,0.0010155977,0.02221415],"study_design_scores_gemma":[0.0000046130026,0.000048459642,0.993105,0.0000035395874,0.0000148343715,0.00068345404,0.00027089,0.0007908813,0.0038995254,0.000029276634,0.001146961,0.0000025916015],"about_ca_topic_score_codex":0.002519741,"about_ca_topic_score_gemma":0.0076156617,"teacher_disagreement_score":0.002519741,"about_ca_system_score_codex":0.00013355761,"about_ca_system_score_gemma":0.00007030427,"threshold_uncertainty_score":0.005010128},"labels":[],"label_agreement":null},{"id":"W4281262570","doi":"10.3847/1538-4357/ac649f","title":"Disks in Nearby Young Stellar Associations Found Via Virtual Reality","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"","keywords":"Physics; Argus; Stars; Vega; Astrophysics; Luminosity; Debris disk; Population; Astronomy; Computer science; Planetary system; Medicine; Galaxy","score_opus":0.01731086118988917,"score_gpt":0.2504794436322825,"score_spread":0.2331685824423933,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281262570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984578,0.000022523958,0.0006620908,0.000012849636,0.000001506117,0.00000709652,0.00013009406,0.000022661789,0.00068330654],"genre_scores_gemma":[0.9990159,0.000010959224,0.0007343232,0.000002998821,0.0000012105314,0.000004527631,0.0001156999,0.000002026522,0.00011226914],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997061,0.00008919034,0.000013605499,0.00007069896,0.000068365174,0.000051943356],"domain_scores_gemma":[0.9992913,0.00022295615,0.00019341434,0.000107693595,0.00007260471,0.00011201715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036458817,0.0001338765,0.00016654396,0.0018540466,0.00036469573,0.0011675011,0.00024125901,0.00022345067,0.0013961331],"category_scores_gemma":[0.0014820062,0.0001171087,0.0001652995,0.0008596912,0.0002874194,0.00044539757,0.0013195737,0.00014789318,0.00013885865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007193,0.00020874951,0.8983294,0.000098424585,0.00010765147,0.0009428611,0.010178365,0.003161671,0.015593251,0.00097279064,0.0009521637,0.0687354],"study_design_scores_gemma":[0.000024288067,0.00021315254,0.96131027,0.00003299012,0.00007816081,0.0009289341,0.013521977,0.014758318,0.002773815,0.00068516925,0.0056409393,0.0000319278],"about_ca_topic_score_codex":0.005930569,"about_ca_topic_score_gemma":0.0075415783,"teacher_disagreement_score":0.005930569,"about_ca_system_score_codex":0.00028800475,"about_ca_system_score_gemma":0.00013684321,"threshold_uncertainty_score":0.011792123},"labels":[],"label_agreement":null},{"id":"W4281264359","doi":"10.3847/1538-4357/ac7051","title":"Resolved Stellar Mass Maps of Galaxies in the Hubble Frontier Fields: Evidence for Mass Dependency in Environmental Quenching","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; McGill University; Herzberg Institute of Astrophysics; University of Toronto; York University","funders":"","keywords":"Physics; Astrophysics; Bulge; Galaxy; Stellar mass; Astronomy; Elliptical galaxy; Galaxy cluster; Ram pressure; Population; Star formation","score_opus":0.014600167644696353,"score_gpt":0.22625100876797488,"score_spread":0.21165084112327853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281264359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988716,0.000035195648,0.0004563053,0.000007846624,3.582775e-7,0.000002078484,0.00008928364,0.00002359724,0.00051373825],"genre_scores_gemma":[0.9997149,0.0000079310175,0.00013879241,0.0000035880219,0.0000012699205,8.829849e-7,0.00008154113,0.0000027101712,0.00004826275],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999002,0.0000105647005,0.0000044256253,0.00003478575,0.000026866708,0.000023183686],"domain_scores_gemma":[0.9989411,0.00026747736,0.00035259634,0.00012434793,0.00011362139,0.00020086368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003161857,0.00015788907,0.00016928562,0.0015512634,0.00016083985,0.00038193926,0.00028240998,0.00019620454,0.0009873036],"category_scores_gemma":[0.0010138443,0.00015652589,0.00016432235,0.00040883935,0.00036483433,0.0003546204,0.00032818416,0.00013101543,0.00018414346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015535142,0.000053038242,0.95707244,0.000021195974,0.000059837355,0.00009837683,0.00024150082,0.0029289343,0.030869506,0.0005108164,0.00012951522,0.007859429],"study_design_scores_gemma":[0.0000021832132,0.000011707903,0.9972012,0.0000012345582,0.0000038673643,0.000024388033,0.000028314878,0.0019081548,0.0006691326,0.00009206503,0.00005570851,0.0000019770882],"about_ca_topic_score_codex":0.0023139787,"about_ca_topic_score_gemma":0.002181613,"teacher_disagreement_score":0.0023139787,"about_ca_system_score_codex":0.00024886162,"about_ca_system_score_gemma":0.00006689815,"threshold_uncertainty_score":0.0046010017},"labels":[],"label_agreement":null},{"id":"W4281389325","doi":"10.3847/1538-4357/ac7f9c","title":"Pre-supernova Alert System for Super-Kamiokande","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg; British Columbia Institute of Technology; TRIUMF; University of Toronto","funders":"Ministry of Education, Culture, Sports, Science and Technology; Japan Society for the Promotion of Science; Horizon 2020 Framework Programme; Kerman Neuroscience Research Center, Kerman University of Medical Sciences; Science and Technology Facilities Council; National Research Foundation; Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; European Commission; Western Canada Research Grid; National Natural Science Foundation of China; National Science Foundation; Compute Canada; National Research Foundation of Korea","keywords":"Neutrino; Supernova; Physics; Neutrino detector; Astrophysics; Super-Kamiokande; Stars; Astronomy; Nuclear physics; Solar neutrino; Neutrino oscillation","score_opus":0.019339342190395643,"score_gpt":0.2811573170336927,"score_spread":0.26181797484329705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281389325","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5971371,0.0020379806,0.24908568,0.0016066468,0.00092457066,0.0014273775,0.0076276716,0.106180094,0.033972953],"genre_scores_gemma":[0.88709706,0.00017036377,0.09794795,0.00052525353,0.00015358724,0.00029340005,0.0040159062,0.0006518788,0.009144612],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9995432,0.00007230029,0.000034709716,0.00012943476,0.00013858051,0.0000817983],"domain_scores_gemma":[0.99843377,0.00022020839,0.00019502312,0.00030185527,0.00056931336,0.00027981447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016484398,0.0005140829,0.00041330152,0.001708497,0.00038261036,0.00080038555,0.00075605017,0.00077036174,0.005881292],"category_scores_gemma":[0.0018171187,0.00028045123,0.00026352986,0.00044647412,0.00020572593,0.0008461831,0.0013065906,0.0006728781,0.0030822312],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.006769553,0.0005686266,0.19427109,0.0006428699,0.00028358758,0.0022939325,0.0014340517,0.0035327664,0.37403968,0.008261926,0.04336196,0.36453998],"study_design_scores_gemma":[0.0006853801,0.0026647935,0.18034787,0.00021734137,0.00040001608,0.0026392387,0.0005391945,0.13682112,0.44287252,0.0072364267,0.22528993,0.00028610986],"about_ca_topic_score_codex":0.0008332978,"about_ca_topic_score_gemma":0.0009912603,"teacher_disagreement_score":0.005881292,"about_ca_system_score_codex":0.0004879271,"about_ca_system_score_gemma":0.0004616184,"threshold_uncertainty_score":0.019674838},"labels":[],"label_agreement":null},{"id":"W4281477531","doi":"10.3847/1538-4357/ac9785","title":"Searches for Neutrinos from Gamma-Ray Bursts Using the IceCube Neutrino Observatory","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; U.S. Department of Energy; University of Wisconsin-Madison; Vetenskapsrådet; National Research Foundation; Michigan State University; University of Oxford; Compute Canada; Marquette University; Fonds Wetenschappelijk Onderzoek; National Aeronautics and Space Administration","keywords":"Physics; Neutrino; Neutrino astronomy; Astrophysics; Cosmic ray; Flux (metallurgy); Neutrino detector; Solar neutrino problem; Gamma-ray burst; Muon; Cosmic neutrino background; COSMIC cancer database; Observatory; Solar neutrino; Measurements of neutrino speed; Astronomy; Neutrino oscillation; Particle physics","score_opus":0.037431623997003,"score_gpt":0.25813678844217613,"score_spread":0.22070516444517313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281477531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97911215,0.00033839062,0.0032723583,0.0000727878,0.000018171091,0.000097730306,0.010835742,0.00017087924,0.0060818046],"genre_scores_gemma":[0.95814013,0.00060400873,0.012436623,0.00005078733,0.000031938132,0.00015209915,0.027494663,0.000058088637,0.0010316292],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997799,0.000055921373,0.000013050501,0.00006666469,0.00005394204,0.000030537187],"domain_scores_gemma":[0.9994149,0.0001593704,0.00020166872,0.000092613576,0.000065822715,0.000065686516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062250276,0.00047410847,0.00036327948,0.0012604959,0.00039256722,0.0009618634,0.00027610763,0.0002136338,0.0012298819],"category_scores_gemma":[0.00079187774,0.00017915656,0.00044687476,0.0014062311,0.0001678855,0.00027951988,0.0007085165,0.00026783525,0.0002128155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0033345218,0.00024176687,0.8342796,0.00024464403,0.00061791966,0.0006097142,0.00048115756,0.008265163,0.08470038,0.0024961152,0.005172547,0.059556432],"study_design_scores_gemma":[0.00017484232,0.00036026482,0.92922485,0.00008475587,0.00030412542,0.0005993289,0.00034118476,0.014317949,0.029330743,0.0015996972,0.023617733,0.00004457074],"about_ca_topic_score_codex":0.004390337,"about_ca_topic_score_gemma":0.007492238,"teacher_disagreement_score":0.004390337,"about_ca_system_score_codex":0.00031042963,"about_ca_system_score_gemma":0.0004966053,"threshold_uncertainty_score":0.008729577},"labels":[],"label_agreement":null},{"id":"W4281555091","doi":"10.3847/1538-4357/ac64a4","title":"Grain Alignment in the Circumstellar Shell of IRC+10° 216","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Science Foundation","keywords":"Physics; Cosmic dust; Astrophysics; Polarization (electrochemistry); Diamagnetism; Interstellar medium; Paramagnetism; Radiative transfer; Polarimetry; Infrared; Astronomy; Magnetic field; Optics; Scattering; Condensed matter physics","score_opus":0.010992237425752253,"score_gpt":0.23043341107747822,"score_spread":0.21944117365172597,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281555091","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990134,0.000017360777,0.0000769152,0.000004351268,0.0000013190446,0.0000015762855,0.00020985247,0.000012071166,0.00066312763],"genre_scores_gemma":[0.9992269,0.000009876941,0.00013295334,0.000007034378,0.0000017515127,0.0000012780657,0.0004955126,0.000006588026,0.00011804372],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999167,0.0000037329796,0.0000037385444,0.000035358866,0.000017869392,0.000022689144],"domain_scores_gemma":[0.9998437,0.000009550691,0.000049768434,0.000021188185,0.0000348021,0.000040893872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006353746,0.0001773999,0.00015241317,0.0004953541,0.00035653258,0.0004622822,0.00019819006,0.0002507862,0.0010916174],"category_scores_gemma":[0.00014303956,0.00013237038,0.0000994658,0.00035458204,0.00017738705,0.000118457,0.00027995222,0.00018184674,0.00034452885],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046150514,0.00007393419,0.30397406,0.000032709097,0.00003089263,0.0004239305,0.0001350094,0.00053749117,0.68764573,0.00012616116,0.00022322977,0.0063354014],"study_design_scores_gemma":[0.0000080865375,0.00004695273,0.98493075,0.0000023662544,0.000008064765,0.00015405708,0.000096331,0.000576412,0.013716438,0.000027977938,0.00042899323,0.0000035046894],"about_ca_topic_score_codex":0.0042401436,"about_ca_topic_score_gemma":0.004081463,"teacher_disagreement_score":0.0042401436,"about_ca_system_score_codex":0.00028722736,"about_ca_system_score_gemma":0.00010421393,"threshold_uncertainty_score":0.008430958},"labels":[],"label_agreement":null},{"id":"W4281557013","doi":"10.3847/1538-4357/ac69d7","title":"The SDSS-HET Survey of Kepler Eclipsing Binaries. A Sample of Four Benchmark Binaries","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Science Mission Directorate; Nuclear Safety and Security Commission; Georg-August-Universität Göttingen; York University; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Spectrograph; Physics; Sky; Astrophysics; Kepler; Benchmark (surveying); RADIUS; Radial velocity; Astronomy; Stars; Spectral line; Computer science; Geodesy; Geology","score_opus":0.02433129453850055,"score_gpt":0.23852419315344586,"score_spread":0.2141928986149453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281557013","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960141,0.00017819091,0.0002327845,0.000015872034,0.0000020908776,0.000011487464,0.0023255597,0.000020067726,0.0011997801],"genre_scores_gemma":[0.98929274,0.00008645129,0.00048609148,0.000018750936,0.000004904305,0.000009879457,0.0097138,0.000013212888,0.00037404647],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999742,0.000041014962,0.000025826695,0.000077249926,0.00006388006,0.000050050887],"domain_scores_gemma":[0.9990871,0.00009327633,0.00029612923,0.00016163714,0.00013599417,0.00022593861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050281314,0.0002664334,0.0002543016,0.0019114917,0.00036325955,0.00047713675,0.00029781248,0.00019506145,0.00079084013],"category_scores_gemma":[0.0013634663,0.00015237073,0.000106403706,0.0013376907,0.0001902587,0.00051564374,0.0008985393,0.00013767327,0.00057238207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029437692,0.000065363056,0.98200226,0.000026105869,0.000039706298,0.00009305889,0.00018791546,0.0008038632,0.0039484394,0.00035099784,0.0011691161,0.011018751],"study_design_scores_gemma":[0.0000090191415,0.000029254115,0.99636084,0.0000046488726,0.0000073363926,0.00009787493,0.00011404706,0.0009997381,0.00066401367,0.00007698081,0.0016334611,0.0000027566837],"about_ca_topic_score_codex":0.007878119,"about_ca_topic_score_gemma":0.020288523,"teacher_disagreement_score":0.007878119,"about_ca_system_score_codex":0.00045005337,"about_ca_system_score_gemma":0.0002140134,"threshold_uncertainty_score":0.015664518},"labels":[],"label_agreement":null},{"id":"W4281643699","doi":"10.3847/1538-4357/ac6a5d","title":"Exploring Changes in Quasar Spectral Energy Distributions across C iv Parameter Space","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Science Board; National Aeronautics and Space Administration","keywords":"Physics; Quasar; Astrophysics; Blueshift; Spectral line; Astronomy; Galaxy; Optics","score_opus":0.04757579198675222,"score_gpt":0.2571644492589384,"score_spread":0.20958865727218617,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281643699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989729,0.000042596293,0.0004276128,0.0000070681713,5.918858e-7,0.0000014683471,0.00012278027,0.000014910599,0.00041004756],"genre_scores_gemma":[0.9996244,0.000012125614,0.00013978721,0.0000027949031,8.974067e-7,0.000001210323,0.00016148516,0.0000054087477,0.000051799765],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998454,0.000028808065,0.000010389781,0.000054460164,0.000030580977,0.000030280962],"domain_scores_gemma":[0.9986796,0.0005636886,0.0003405571,0.00015353713,0.00015523547,0.00010730708],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053694384,0.00024736894,0.00023274208,0.0019074243,0.00020347915,0.00082931295,0.0002607631,0.0002496066,0.0011581342],"category_scores_gemma":[0.0016744559,0.00014512603,0.00024175155,0.0007095805,0.00036425464,0.00044641047,0.00043663356,0.00034225773,0.0001886391],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000142681,0.00003272718,0.96846485,0.000020587186,0.0001684549,0.00009193002,0.00019754228,0.0050473856,0.015916215,0.00050348643,0.00014285323,0.0092713935],"study_design_scores_gemma":[0.0000039380975,0.00004511063,0.988408,0.0000054928173,0.000020760479,0.00009349841,0.0002871715,0.008526534,0.0019518754,0.00030328144,0.00034033484,0.00001412202],"about_ca_topic_score_codex":0.002064229,"about_ca_topic_score_gemma":0.0015590569,"teacher_disagreement_score":0.002064229,"about_ca_system_score_codex":0.00019967048,"about_ca_system_score_gemma":0.00007757479,"threshold_uncertainty_score":0.0041044354},"labels":[],"label_agreement":null},{"id":"W4281655528","doi":"10.3847/1538-4357/ac722a","title":"The Twisted Magnetic Field of the Protobinary L483","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Queen's University","funders":"","keywords":"Physics; Astrophysics; Magnetic field; Polarization (electrochemistry); Polarimetry; Bipolar outflow; Field (mathematics); Envelope (radar); Stars; Star formation; Optics","score_opus":0.006684232052679235,"score_gpt":0.22836336907252375,"score_spread":0.2216791370198445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281655528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99854565,0.000024252788,0.000093652256,0.00003173693,0.000002108623,0.0000018011618,0.00011054787,0.000021083506,0.0011691466],"genre_scores_gemma":[0.99958295,0.000004672918,0.00009137841,0.00002091897,0.000001954747,0.0000012606107,0.00011436035,0.0000041347903,0.00017843518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995625,0.0000022665636,0.0000014817384,0.00001053588,0.000013534212,0.000015897316],"domain_scores_gemma":[0.99986804,0.000009011778,0.00003486939,0.000013459794,0.000019278626,0.00005527754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005186742,0.00013142772,0.00022720448,0.00039608346,0.0006102136,0.0004080322,0.00024268756,0.00027740054,0.0018601498],"category_scores_gemma":[0.00011661826,0.00010154061,0.0001683438,0.00022764184,0.00030239223,0.00013756371,0.00041512915,0.00033656755,0.00046152595],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078605395,0.00013133649,0.49351436,0.00004427243,0.00006613506,0.0025565173,0.0008517348,0.00062027574,0.48025954,0.00041279985,0.0017328731,0.019024076],"study_design_scores_gemma":[0.000026627367,0.00009258011,0.98954016,0.000007620754,0.000012085211,0.0008809452,0.00033310265,0.0011468196,0.0060852873,0.00019862904,0.0016640312,0.000012154375],"about_ca_topic_score_codex":0.0043132007,"about_ca_topic_score_gemma":0.006997673,"teacher_disagreement_score":0.0043132007,"about_ca_system_score_codex":0.000502678,"about_ca_system_score_gemma":0.00011665563,"threshold_uncertainty_score":0.008576214},"labels":[],"label_agreement":null},{"id":"W4281656095","doi":"10.3847/1538-4357/ac7464","title":"Disks and Outflows in the Intermediate-mass Star-forming Region NGC 2071 IR","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Agencia Estatal de Investigación; European Commission; European Regional Development Fund; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Science and Technology Facilities Council; Consejería de Transformación Económica, Industria, Conocimiento y Universidades; Associated Universities; National Aeronautics and Space Administration; Instituto de Astrofísica de Andalucía; Junta de Andalucía; National Science Foundation","keywords":"Physics; Astrophysics; Protostar; Star formation; Millimeter; Outflow; Bipolar outflow; Submillimeter Array; Astronomy; Galaxy","score_opus":0.013467659771614527,"score_gpt":0.23896213991928927,"score_spread":0.22549448014767476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281656095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993709,0.000027690136,0.00006412389,0.0000067653214,4.4033638e-7,0.0000019807267,0.00007358391,0.000012015635,0.0004424198],"genre_scores_gemma":[0.99948573,0.000021138285,0.00022430914,0.0000072249154,0.0000019735457,0.0000031984173,0.00018029918,0.000002770577,0.000073290925],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999948,0.00000489974,0.0000030336894,0.000014438775,0.000012033219,0.00001759064],"domain_scores_gemma":[0.9997497,0.00005620937,0.00009055547,0.000016790551,0.000019472067,0.00006731013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011498544,0.00013876098,0.00025596275,0.0005430386,0.00057991536,0.00044305983,0.00035393913,0.00027542928,0.00092610816],"category_scores_gemma":[0.00030707192,0.00014801307,0.00014457796,0.00029481598,0.00018364198,0.00016488768,0.00029081138,0.00019273917,0.00018849169],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047354103,0.00021946458,0.9281309,0.0000722423,0.00005698689,0.0016864856,0.00076715805,0.006504837,0.04765238,0.00056198094,0.0006863071,0.0131877195],"study_design_scores_gemma":[0.000013902968,0.0000574442,0.99005777,0.000010632302,0.000019129038,0.00040362365,0.00024982792,0.0072009475,0.001508512,0.00013026851,0.00033907904,0.0000088166225],"about_ca_topic_score_codex":0.0068384935,"about_ca_topic_score_gemma":0.0077579487,"teacher_disagreement_score":0.0068384935,"about_ca_system_score_codex":0.0005026732,"about_ca_system_score_gemma":0.00016374925,"threshold_uncertainty_score":0.013597369},"labels":[],"label_agreement":null},{"id":"W4281675887","doi":"10.3847/1538-4357/ac96ed","title":"Magellan/IMACS Spectroscopy of Grus I: A Low Metallicity Ultra-faint Dwarf Galaxy*","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Natural Sciences and Engineering Research Council of Canada; Institut de Física d'Altes Energies; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Deutsche Forschungsgemeinschaft; University of Portsmouth; University of Chicago; Kavli Institute for Cosmological Physics, University of Chicago; Ohio State University; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; University of Sussex; Ministério da Ciência, Tecnologia e Inovação; University College London; National Aeronautics and Space Administration; Science and Technology Facilities Council; European Space Agency; Brinson Foundation; Fermilab; National Science Foundation; Argonne National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Metallicity; Velocity dispersion; Galaxy; Dwarf galaxy; Milky Way; Grus (genus); Sigma; Astronomy; Population; Medicine","score_opus":0.012511096655658537,"score_gpt":0.24536438445657094,"score_spread":0.2328532878009124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281675887","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976955,0.00006910741,0.00021617384,0.000031012445,0.0000028216573,0.000003719533,0.0003649108,0.000080863116,0.0015358463],"genre_scores_gemma":[0.9978849,0.000031500913,0.0009491936,0.000024316634,0.000011947394,0.0000022716915,0.00065575074,0.000017661987,0.0004224627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990344,0.0000054433594,0.000004400195,0.000033392163,0.00003113774,0.000022146229],"domain_scores_gemma":[0.9997682,0.000011695757,0.00005481621,0.000034120916,0.00004540828,0.00008575855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017595131,0.0002452558,0.0001939378,0.0010639122,0.00030630938,0.00033657235,0.0003719343,0.00019272356,0.0012285209],"category_scores_gemma":[0.00024145369,0.00009189262,0.00014985626,0.0005412955,0.00018268876,0.00019538126,0.00037804226,0.00014956803,0.0005959007],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023088622,0.000071044786,0.80146104,0.00007022245,0.00007810665,0.0004930536,0.0007361941,0.0007713508,0.16025978,0.00059489976,0.00263941,0.032594115],"study_design_scores_gemma":[0.0000062766912,0.00006124954,0.98521847,0.000007987153,0.000025605686,0.00034993503,0.00020702319,0.0012226368,0.009286599,0.000112260794,0.0034939933,0.000007980682],"about_ca_topic_score_codex":0.0036511645,"about_ca_topic_score_gemma":0.006101647,"teacher_disagreement_score":0.0036511645,"about_ca_system_score_codex":0.00031387966,"about_ca_system_score_gemma":0.00008674787,"threshold_uncertainty_score":0.0072598457},"labels":[],"label_agreement":null},{"id":"W4281740477","doi":"10.3847/1538-4357/ac7468","title":"On the Dwarf Irregular Galaxy NGC 6822. I. Young, Intermediate, and Old Stellar Populations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Planetary Science Division; European Regional Development Fund; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Agencia Estatal de Investigación; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of California, Los Angeles; Max-Planck-Institut für Astronomie; National Astronomical Observatory of Japan; Agencia Canaria de Investigación, Innovación y Sociedad de la Información; Toray Science Foundation; High Energy Accelerator Research Organization; Ministerio de Ciencia e Innovación; Max-Planck-Gesellschaft; Cabinet Office, Government of Japan; Space Telescope Science Institute; Los Alamos National Laboratory; European Space Agency; Princeton University; Johns Hopkins University; Jet Propulsion Laboratory; Ministry of Education, Culture, Sports, Science and Technology; National Central University; Gordon and Betty Moore Foundation; National Science Foundation; Eötvös Loránd Tudományegyetem; Academia Sinica; California Institute of Technology; National Aeronautics and Space Administration; Durham University; Japan Science and Technology Agency; Smithsonian Institution","keywords":"Physics; Astrophysics; Galaxy; Local Group; Astronomy; Metallicity; Photometry (optics); Red-giant branch; Stars; Irregular galaxy; Stellar population; Asymptotic giant branch; Population; Carbon star; Dwarf galaxy; Giant star; Red supergiant; Supergiant; Star formation; Interacting galaxy","score_opus":0.010128562293100645,"score_gpt":0.21236565313388236,"score_spread":0.20223709084078173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281740477","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982443,0.00021394418,0.00021646712,0.000009941394,0.0000018172086,0.0000025948518,0.0002116106,0.00002725193,0.0010722181],"genre_scores_gemma":[0.99921083,0.000052754924,0.00030755583,0.000004580375,0.000004341395,0.0000016262387,0.00029701926,0.000004381491,0.0001168512],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988496,0.000015554062,0.0000050821113,0.000033181335,0.00003100052,0.000030153487],"domain_scores_gemma":[0.99965465,0.000038450537,0.00011176993,0.000042600495,0.000060992137,0.00009151029],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001344017,0.00027340502,0.00016938281,0.0011670074,0.0002356572,0.00027929852,0.00018889505,0.0001316378,0.0006817764],"category_scores_gemma":[0.0003737942,0.000077107274,0.00010053428,0.00055754784,0.00021318269,0.00021961976,0.00034423845,0.0000915971,0.00030494106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020202479,0.000026085612,0.9459372,0.000039229522,0.000021875328,0.00028310143,0.00032706084,0.0009770624,0.020230036,0.00028347236,0.00059434597,0.031078497],"study_design_scores_gemma":[0.0000030441952,0.000045917015,0.99701226,0.000008388844,0.000008485917,0.00016403403,0.000082482286,0.0008397365,0.0006378203,0.000064242966,0.0011301539,0.000003500534],"about_ca_topic_score_codex":0.006771371,"about_ca_topic_score_gemma":0.014671415,"teacher_disagreement_score":0.006771371,"about_ca_system_score_codex":0.0002870869,"about_ca_system_score_gemma":0.000061336694,"threshold_uncertainty_score":0.013463914},"labels":[],"label_agreement":null},{"id":"W4281751471","doi":"10.3847/1538-4357/ac74c2","title":"Eta Carinae: An Evolving View of the Central Binary, Its Interacting Winds and Its Foreground Ejecta","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Ejecta; Line (geometry); Line-of-sight; Spectral line; Binary number; Wind speed; Ionization; Flux (metallurgy); Orbital period; Extinction (optical mineralogy); Primary (astronomy); Astronomy; Meteorology; Stars; Geometry; Optics; Chemistry","score_opus":0.015963392371832502,"score_gpt":0.2540442442071073,"score_spread":0.2380808518352748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281751471","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93790025,0.039691076,0.00096629956,0.0022285504,0.000091430746,0.000009694729,0.00016897776,0.000040867944,0.018902754],"genre_scores_gemma":[0.98834074,0.008528137,0.0006303373,0.00021379268,0.00020344129,0.0000038149715,0.00010670195,0.000010273132,0.0019627842],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999168,0.000012909148,0.0000039830697,0.00002741635,0.000019488809,0.000019561672],"domain_scores_gemma":[0.99980754,0.000034328514,0.00004130448,0.000008828482,0.000046721427,0.00006125026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029052264,0.00017342139,0.00020680368,0.0015341772,0.00060183933,0.0018122457,0.00043512878,0.00068983476,0.0017788283],"category_scores_gemma":[0.0003329285,0.000121585814,0.00008977748,0.000792131,0.00086005655,0.0014938327,0.0006296965,0.00051987194,0.00029404517],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000762726,0.00016703302,0.5893056,0.0008051952,0.00015031976,0.006636307,0.011198117,0.0014847259,0.05911245,0.012149397,0.0049351,0.313293],"study_design_scores_gemma":[0.0000062512386,0.0001464153,0.91031593,0.00016326892,0.00005034553,0.005895236,0.007757596,0.0013002647,0.0012531838,0.0028884686,0.070194505,0.000028442102],"about_ca_topic_score_codex":0.009428225,"about_ca_topic_score_gemma":0.016218232,"teacher_disagreement_score":0.009428225,"about_ca_system_score_codex":0.0009518476,"about_ca_system_score_gemma":0.0003282048,"threshold_uncertainty_score":0.018746734},"labels":[],"label_agreement":null},{"id":"W4281802380","doi":"10.3847/1538-4357/ac76c7","title":"On the Nature of Ultracool White Dwarfs: Not so Cool after All","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Victoria; Université de Montréal","funders":"","keywords":"White dwarf; Physics; Astrophysics; Brown dwarf; Massive compact halo object; Atmosphere (unit); White (mutation); Astronomy; Stars; Chemistry; Meteorology","score_opus":0.007072113374595078,"score_gpt":0.2164788398916648,"score_spread":0.20940672651706974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281802380","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970196,0.00054966076,0.001087213,0.000102837,0.0000054027423,0.0000021912128,0.00016414102,0.00003428232,0.001034687],"genre_scores_gemma":[0.9991303,0.00015035109,0.00022892792,0.000031964737,0.000009841725,0.0000010516136,0.00021513582,0.0000129195905,0.0002195209],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979645,0.000019313718,0.000005977072,0.00007186237,0.000056633915,0.000049847302],"domain_scores_gemma":[0.99942076,0.00009311521,0.00016534708,0.000093298135,0.000065363696,0.00016212485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035035991,0.00015640892,0.00034398405,0.00059236714,0.000513742,0.0010447531,0.00038765755,0.00012446998,0.000616126],"category_scores_gemma":[0.0008617928,0.00007833354,0.0001419673,0.0006534309,0.00075612834,0.00041414023,0.00047325372,0.00019588508,0.00020090798],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013713024,0.000021673413,0.96600026,0.00003806484,0.000053657506,0.00025423567,0.0007947567,0.000545578,0.010859007,0.0033073484,0.0006312766,0.017356979],"study_design_scores_gemma":[0.0000059976746,0.000037707516,0.9879367,0.000013612949,0.000026122696,0.00029140958,0.0005893508,0.0016881014,0.0031680244,0.0024497109,0.0037818784,0.000011368145],"about_ca_topic_score_codex":0.008522868,"about_ca_topic_score_gemma":0.0135029815,"teacher_disagreement_score":0.008522868,"about_ca_system_score_codex":0.00040924354,"about_ca_system_score_gemma":0.00025751884,"threshold_uncertainty_score":0.016946495},"labels":[],"label_agreement":null},{"id":"W4281860112","doi":"10.3847/1538-4357/ac6096","title":"The Compact Structures of Massive z ∼ 0.7 Post-starburst Galaxies in the SQuIGGLE Sample","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Ohio State University; University of Tokyo; High Energy Accelerator Research Organization; York University; Carnegie Mellon University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Yale University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Vanderbilt University; University of Arizona; Brookhaven National Laboratory; Academia Sinica; U.S. Department of Energy","keywords":"Physics; Galaxy; Astrophysics; Sample (material); Astronomy; Luminous infrared galaxy","score_opus":0.007918612243636472,"score_gpt":0.22133919968397708,"score_spread":0.21342058744034062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281860112","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999318,0.000032956457,0.00006064395,0.000009811988,5.600353e-7,0.000001665883,0.00019580382,0.000010615564,0.0003699026],"genre_scores_gemma":[0.9991109,0.000014283831,0.00007988321,0.0000117648515,0.0000024514784,0.0000015394439,0.00053108484,0.0000042512866,0.00024381862],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998678,0.000012014137,0.000008911577,0.000046297537,0.00002481307,0.000040131654],"domain_scores_gemma":[0.9989466,0.00010436312,0.00030092068,0.00017107709,0.00011980591,0.00035729833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030790947,0.00020371076,0.000224693,0.0013909182,0.00028514498,0.00060241064,0.00029546514,0.00014540709,0.0021255235],"category_scores_gemma":[0.00083164306,0.00013964738,0.00021589754,0.0003987542,0.00041484172,0.00038266947,0.0008765311,0.00020599405,0.00057798874],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013002558,0.00002436728,0.97887117,0.000011333653,0.000033790828,0.00007453679,0.0008485358,0.000056826077,0.014994633,0.000086415384,0.00021188323,0.0046563954],"study_design_scores_gemma":[0.000001494675,0.000021963082,0.99911934,0.0000013242907,0.000005373407,0.000053617896,0.00014170949,0.000048975497,0.00043526612,0.000015486934,0.00015372476,0.0000016403304],"about_ca_topic_score_codex":0.005724555,"about_ca_topic_score_gemma":0.014290368,"teacher_disagreement_score":0.005724555,"about_ca_system_score_codex":0.00019280076,"about_ca_system_score_gemma":0.00008597712,"threshold_uncertainty_score":0.011382461},"labels":[],"label_agreement":null},{"id":"W4281926825","doi":"10.3847/1538-4357/ac71af","title":"3D-DASH: The Widest Near-infrared Hubble Space Telescope Survey","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; York University; University of Toronto","funders":"Space Telescope Science Institute","keywords":"Physics; Astronomy; Hubble space telescope; Hubble Ultra-Deep Field; Space observatory; Hubble Deep Field; Infrared; Hubble Deep Field South; Observational cosmology; Infrared astronomy; Spitzer Space Telescope; Astrophysics; Telescope; Stars; Galaxy; Redshift","score_opus":0.015087980597951467,"score_gpt":0.22673525664723163,"score_spread":0.21164727604928016,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281926825","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.22884414,0.0007913355,0.018205673,0.00058513024,0.00030015348,0.0004225607,0.6978323,0.008832293,0.044186365],"genre_scores_gemma":[0.24539271,0.00046637835,0.035986826,0.0005118431,0.00025701927,0.00045237376,0.6973472,0.0014420479,0.018143516],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.999579,0.00003861423,0.000014846846,0.00011497349,0.00017853797,0.000074058866],"domain_scores_gemma":[0.9991454,0.00003620024,0.000144518,0.0001791226,0.0001946231,0.00030013817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00080657844,0.0005912112,0.0004945766,0.0019335966,0.000414391,0.0006804998,0.00061717065,0.00029501505,0.011272003],"category_scores_gemma":[0.0008188245,0.000219281,0.0004383284,0.001626021,0.00016298161,0.0004951103,0.0011191346,0.0005547981,0.008197065],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001157304,0.00033586513,0.21788573,0.00026953427,0.0002543723,0.00038650725,0.00028265716,0.0037308885,0.019570338,0.0034710893,0.5551914,0.19746436],"study_design_scores_gemma":[0.00024378183,0.000120458026,0.6066932,0.00008810394,0.000051668027,0.00022354811,0.00015336525,0.007629481,0.0034578322,0.0024864892,0.3787825,0.00006953714],"about_ca_topic_score_codex":0.01966042,"about_ca_topic_score_gemma":0.025093403,"teacher_disagreement_score":0.01966042,"about_ca_system_score_codex":0.0005767854,"about_ca_system_score_gemma":0.0010366663,"threshold_uncertainty_score":0.039091945},"labels":[],"label_agreement":null},{"id":"W4281958650","doi":"10.3847/1538-4357/ac75b4","title":"The Size–Mass Relation of Post-starburst Galaxies in the Local Universe","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Chinese Academy of Sciences; National Natural Science Foundation of China; York University; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; China Postdoctoral Science Foundation; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Galaxy; Redshift; Stellar mass; Sky; Star formation; Galaxy formation and evolution; Quenching (fluorescence); Universe; Local Group; Luminous infrared galaxy; Astronomy; Dwarf galaxy","score_opus":0.004966765852755918,"score_gpt":0.19191480454931947,"score_spread":0.18694803869656357,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281958650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993761,0.00007290882,0.00006484502,0.000020169868,4.936387e-7,0.0000011029164,0.00014723367,0.000009419804,0.00030775636],"genre_scores_gemma":[0.9996841,0.000017399125,0.000024985806,0.0000030542137,0.0000018747469,8.4765963e-7,0.00017305817,0.0000020609416,0.00009259427],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987984,0.000016863736,0.0000049167475,0.000039616836,0.00002287585,0.000035842204],"domain_scores_gemma":[0.99796605,0.00043497686,0.0006875957,0.0001646171,0.00028684584,0.0004599532],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003380347,0.00013688655,0.00022661127,0.0013625518,0.0002918146,0.0005347818,0.0003157378,0.00022124355,0.0021839424],"category_scores_gemma":[0.001775073,0.00012218553,0.00020896038,0.00081594463,0.00033697867,0.00041180057,0.00039120702,0.00020436129,0.0003977178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000646649,0.00001511635,0.9932829,0.000009082521,0.000024582281,0.00007693411,0.00028997526,0.00037976418,0.0034348546,0.00021648993,0.00013131429,0.0020743685],"study_design_scores_gemma":[6.8397014e-7,0.00000977402,0.9993414,5.2218985e-7,0.0000024524018,0.000027279177,0.000053882504,0.00035395866,0.000110223365,0.000026218895,0.00007214175,0.0000013205615],"about_ca_topic_score_codex":0.010468616,"about_ca_topic_score_gemma":0.008528866,"teacher_disagreement_score":0.010468616,"about_ca_system_score_codex":0.00046524435,"about_ca_system_score_gemma":0.00011446133,"threshold_uncertainty_score":0.020815313},"labels":[],"label_agreement":null},{"id":"W4281967753","doi":"10.3847/1538-4357/ac7048","title":"SDSS-IV MaNGA: How the Stellar Populations of Passive Central Galaxies Depend on Stellar and Halo Mass","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Vanderbilt University; Consejo Nacional de Ciencia y Tecnología; University of Oxford; York University; Carnegie Institution for Science; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; University of California, Santa Cruz; Ohio State University; U.S. Department of Energy; Smithsonian Institution; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; University of Portsmouth; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Galaxy; Astrophysics; Halo; Physics; Stellar mass; Sigma; Astronomy; Star formation","score_opus":0.01201091358756884,"score_gpt":0.2082413327416789,"score_spread":0.19623041915411005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4281967753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981528,0.00008297339,0.0003572201,0.000022426104,0.0000026295734,0.0000030838319,0.0007591162,0.000098904085,0.0005208704],"genre_scores_gemma":[0.9981192,0.000013979834,0.00041434963,0.000010445956,0.0000043387868,0.0000028442846,0.0012389459,0.00003315927,0.0001627722],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997545,0.000049669212,0.0000112416055,0.00010725224,0.000035938436,0.00004143485],"domain_scores_gemma":[0.9988563,0.00026236012,0.00029138025,0.00021379582,0.00017090996,0.00020527041],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00083129806,0.00027403657,0.00029839482,0.0013218139,0.00024832526,0.00065266126,0.0002931609,0.00015486538,0.0009333987],"category_scores_gemma":[0.0014447379,0.00022497532,0.00036881425,0.0006692108,0.00035632105,0.00038871163,0.00044414046,0.00015218808,0.00050382107],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015784922,0.000024193738,0.97868115,0.00002793878,0.000121510384,0.00005943029,0.00022492098,0.0019727456,0.011858281,0.00024705703,0.0007083426,0.0059166374],"study_design_scores_gemma":[0.0000046672785,0.000015332664,0.9915941,0.0000045968827,0.000018153423,0.00003396018,0.00007147361,0.006758015,0.0009902875,0.00008760972,0.00041614458,0.000005660813],"about_ca_topic_score_codex":0.004596756,"about_ca_topic_score_gemma":0.0051440382,"teacher_disagreement_score":0.004596756,"about_ca_system_score_codex":0.00025910066,"about_ca_system_score_gemma":0.00013106654,"threshold_uncertainty_score":0.009140015},"labels":[],"label_agreement":null},{"id":"W4282046799","doi":"10.3847/1538-4357/ac7e50","title":"The Physical Properties of Low-redshift FeLoBAL Quasars. II. The Rest-frame Optical Emission Line Properties","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; Western University","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; York University; Universität Basel; Fermilab; National Science Foundation; Case Western Reserve University; Carnegie Mellon University; University of Pittsburgh; Los Alamos National Laboratory; College of Engineering, Michigan State University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Princeton University; Aspen Center for Physics; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Drexel University; Vanderbilt University; University of Oklahoma; National Aeronautics and Space Administration; U.S. Naval Observatory; U.S. Department of Energy","keywords":"Quasar; Astrophysics; Physics; Redshift; Emission spectrum; Rest frame; Line (geometry); OVV quasar; Astronomy; Galaxy; Spectral line","score_opus":0.012424658292567321,"score_gpt":0.2161313545543922,"score_spread":0.2037066962618249,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4282046799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951315,0.000064988264,0.000048528753,0.0000047966873,4.476621e-7,0.0000020622997,0.00015498085,0.000002675654,0.000208374],"genre_scores_gemma":[0.99949324,0.000027623308,0.000051026673,0.0000051571883,0.0000018891964,0.000001953025,0.00031781607,0.0000014422226,0.00009967687],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998124,0.000023962995,0.000016932376,0.00004706942,0.000043573218,0.000055983066],"domain_scores_gemma":[0.9988286,0.00021621429,0.0005749448,0.00007410666,0.0001300125,0.00017607676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038556466,0.00022637931,0.00025717312,0.0021458757,0.00033490348,0.0006398055,0.0002537373,0.00024249511,0.0013650742],"category_scores_gemma":[0.0013268283,0.00010520903,0.00017084817,0.0008021066,0.0004196585,0.00031877813,0.00035542133,0.00018313016,0.00034580776],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037142156,0.00002224515,0.99236953,0.000009926679,0.000013828778,0.000061348765,0.000104371116,0.000034778277,0.0052931514,0.000031782343,0.00002760271,0.001994383],"study_design_scores_gemma":[7.23289e-7,0.000021895255,0.9994536,9.809395e-7,0.0000031700222,0.00010071807,0.00006215876,0.00003404804,0.0002355262,0.00001134193,0.00007487245,0.0000010531052],"about_ca_topic_score_codex":0.0020025172,"about_ca_topic_score_gemma":0.0022302151,"teacher_disagreement_score":0.0021458757,"about_ca_system_score_codex":0.0002119391,"about_ca_system_score_gemma":0.000063339634,"threshold_uncertainty_score":0.00456661},"labels":[],"label_agreement":null},{"id":"W4282959171","doi":"10.3847/1538-4357/ac6de6","title":"Circumnuclear Medium around the Central AGN in a Cool-core Cluster, Abell 1644-South","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"National Institutes of Natural Sciences; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; National Research Foundation of Korea; Canadian Space Agency; National Research Foundation; National Science Foundation; Korea Astronomy and Space Science Institute; Yonsei University; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Intracluster medium; Active galactic nucleus; Galaxy cluster; Galaxy; Astronomy; Redshift; Cluster (spacecraft); Cooling flow; Radiative cooling; Virgo Cluster","score_opus":0.01020489290522073,"score_gpt":0.2069236947038251,"score_spread":0.19671880179860438,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4282959171","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993765,0.00005799677,0.000038345228,0.000009120184,0.0000021525962,0.0000015960136,0.00017639947,0.000009985221,0.0003279026],"genre_scores_gemma":[0.9993075,0.00002062793,0.000077626144,0.0000059396825,0.000004363954,0.0000015210131,0.00039327855,0.0000024507524,0.00018668504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994886,0.0000027738654,0.0000019531888,0.000015155447,0.000009393142,0.000021836273],"domain_scores_gemma":[0.99983275,0.00001089069,0.000058212026,0.000008461657,0.00001967567,0.00007005484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005494594,0.00016167232,0.00020386891,0.0010497046,0.0005189906,0.00043317516,0.00019018978,0.00017053065,0.0010271927],"category_scores_gemma":[0.00013447655,0.00009704431,0.000112454676,0.00043303974,0.0001868693,0.00018212835,0.0003526053,0.00010394656,0.00018909524],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041440869,0.0001139974,0.86728716,0.000038018035,0.000077510645,0.0016683558,0.00042834296,0.001213617,0.12200441,0.0002214551,0.00081044674,0.005722184],"study_design_scores_gemma":[0.00000426168,0.00002754158,0.997719,0.0000016829464,0.000010087284,0.000116259434,0.00013807454,0.00054924825,0.0010254254,0.00002573823,0.0003790572,0.000003598578],"about_ca_topic_score_codex":0.019315062,"about_ca_topic_score_gemma":0.025776291,"teacher_disagreement_score":0.019315062,"about_ca_system_score_codex":0.00039692898,"about_ca_system_score_gemma":0.00015687283,"threshold_uncertainty_score":0.0384053},"labels":[],"label_agreement":null},{"id":"W4282961335","doi":"10.3847/1538-4357/ac8e04","title":"The Pantheon+ Analysis: Cosmological Constraints","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1221,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Science and Technology Facilities Council","keywords":"Physics; Cosmic microwave background; Dark energy; Baryon acoustic oscillations; Redshift; Astrophysics; Baryon; Omega; Cepheid variable; Supernova; Cosmological constant; Hubble's law; Cosmic background radiation; Spectral density; Cosmology; Lambda; Universe; Galaxy; Mathematical physics; Statistics","score_opus":0.01198267423743017,"score_gpt":0.23490231282829344,"score_spread":0.22291963859086328,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4282961335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86938536,0.0005689235,0.048710667,0.0012338681,0.000059535367,0.000037548736,0.007601416,0.0008613573,0.07154141],"genre_scores_gemma":[0.98424387,0.000089825015,0.009131855,0.00011674948,0.0000310933,0.00001744146,0.0015265476,0.00014749513,0.004695226],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99827313,0.0010022493,0.000038508068,0.0003160016,0.00022832245,0.00014165185],"domain_scores_gemma":[0.9970535,0.001711933,0.0004147837,0.00044706013,0.0002787141,0.000093912604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011947675,0.00046432234,0.00040242902,0.0015120936,0.0006082252,0.0010470604,0.0004702595,0.00019538126,0.01590622],"category_scores_gemma":[0.0044965055,0.00019265541,0.00039147056,0.0015960186,0.00038942767,0.00060260907,0.0009882094,0.0003235253,0.00093440025],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001605206,0.00008800741,0.6632685,0.0003738715,0.0008855647,0.0014791102,0.0006662868,0.021774951,0.010639538,0.09586037,0.042702064,0.16065656],"study_design_scores_gemma":[0.0001132141,0.00023121924,0.69633025,0.00010667855,0.00037225313,0.0012607989,0.0005691658,0.13650444,0.009200591,0.06313711,0.09206929,0.000104921244],"about_ca_topic_score_codex":0.009712117,"about_ca_topic_score_gemma":0.017916052,"teacher_disagreement_score":0.01590622,"about_ca_system_score_codex":0.0004820068,"about_ca_system_score_gemma":0.0005514433,"threshold_uncertainty_score":0.05321157},"labels":[],"label_agreement":null},{"id":"W4282970969","doi":"10.3847/1538-4357/ac77e7","title":"Chemical and Physical Characterization of the Isolated Protostellar Source CB68: FAUST IV","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Japan Society for the Promotion of Science","keywords":"Protostar; Astrophysics; Physics; Submillimeter Array; Context (archaeology); RADIUS; Millimeter; Astrochemistry; Interstellar medium; Star formation; Stars","score_opus":0.005709264313183387,"score_gpt":0.20357846250691639,"score_spread":0.197869198193733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4282970969","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991431,0.00009550478,0.000087856846,0.00001094204,0.0000012157417,0.00000411146,0.00021989898,0.00002567977,0.00041168235],"genre_scores_gemma":[0.99923706,0.000023294373,0.00021029617,0.000008075856,0.0000025206602,0.0000030680424,0.0003867348,0.0000070218616,0.00012198327],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996054,0.000001390243,8.2178667e-7,0.000013851711,0.0000091284555,0.000014220673],"domain_scores_gemma":[0.9998404,0.000010361904,0.000049137627,0.000009965535,0.000023344164,0.0000667422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000034143784,0.00029687386,0.00018746055,0.0012263532,0.00039056162,0.0002880292,0.0003096487,0.00018424023,0.0010956874],"category_scores_gemma":[0.0001294405,0.0001085435,0.000103168015,0.0004638612,0.00024745928,0.00011917303,0.00026632447,0.00023436095,0.00021512985],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028709584,0.00010267323,0.4648314,0.00006755601,0.000056066285,0.0009192666,0.00030949624,0.0008672632,0.5213002,0.00014194401,0.0005664798,0.010550622],"study_design_scores_gemma":[0.000010438529,0.000050620387,0.98995346,0.0000062622244,0.000016164735,0.0002695464,0.00012473266,0.0012932713,0.0073924,0.00002976736,0.00084654,0.0000067955516],"about_ca_topic_score_codex":0.015144007,"about_ca_topic_score_gemma":0.017043328,"teacher_disagreement_score":0.015144007,"about_ca_system_score_codex":0.00038664407,"about_ca_system_score_gemma":0.00013655047,"threshold_uncertainty_score":0.03011173},"labels":[],"label_agreement":null},{"id":"W4283021297","doi":"10.3847/1538-4357/ac67dc","title":"The Circumstellar Environments of Double-peaked, Calcium-strong Transients 2021gno and 2021inl","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Planetary Science Division; Deutsches Elektronen-Synchrotron; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Stockholms Universitet; Queen's University; National Centre for Supercomputing Applications; Durham University; Northwestern University; National Central University; Villum Fonden; Los Alamos National Laboratory; University of Washington; Johns Hopkins University; National Science Foundation; Gordon and Betty Moore Foundation; Queen's University Belfast; Canadian Institute for Advanced Research; University of Illinois at Urbana-Champaign; Nuclear Safety and Security Commission; Space Telescope Science Institute; W. M. Keck Foundation; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Physics; Astrophysics; Astronomy","score_opus":0.013464796453752093,"score_gpt":0.22475937888562716,"score_spread":0.21129458243187507,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283021297","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99912614,0.00003187924,0.00013766928,0.000008575314,8.12602e-7,0.0000022260317,0.00015211171,0.000024354662,0.00051617465],"genre_scores_gemma":[0.99928397,0.000020830525,0.00012140893,0.0000049634446,0.0000013171575,0.0000021769174,0.00040850116,0.0000074552922,0.00014950124],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999428,0.0000042153592,0.0000024161889,0.000019648243,0.000008698126,0.00002230399],"domain_scores_gemma":[0.9998498,0.000016009924,0.00005741456,0.000011662518,0.000011731434,0.000053424363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009998598,0.00022403411,0.00020858397,0.00055554905,0.00025410042,0.00064736465,0.00024367063,0.00022574779,0.0009147702],"category_scores_gemma":[0.00020127822,0.00016967928,0.0001957723,0.0003041922,0.00018537576,0.00022478706,0.00041649572,0.00012614913,0.00020606261],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006593058,0.00006616776,0.8526314,0.000056327062,0.000067641675,0.0013375997,0.00032258357,0.006728556,0.13179445,0.0005110365,0.0003484034,0.0054764603],"study_design_scores_gemma":[0.000012804006,0.000054861892,0.9831907,0.0000052258474,0.00001767996,0.00025880555,0.0001610059,0.01033952,0.0052281935,0.00008731094,0.0006356506,0.000008225475],"about_ca_topic_score_codex":0.0050180517,"about_ca_topic_score_gemma":0.0053966246,"teacher_disagreement_score":0.0050180517,"about_ca_system_score_codex":0.00045752915,"about_ca_system_score_gemma":0.00011288109,"threshold_uncertainty_score":0.009977698},"labels":[],"label_agreement":null},{"id":"W4283024364","doi":"10.3847/1538-4357/ac6e3f","title":"ALMA Lensing Cluster Survey: ALMA-Herschel Joint Study of Lensed Dusty Star-forming Galaxies across z ≃ 0.5 – 6","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; Science and Technology Facilities Council; National Astronomical Observatory of Japan; National Science Foundation; Ministry of Science and Technology, Israel; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Luminous infrared galaxy; Star formation; Gravitational lens; Galaxy cluster; Redshift","score_opus":0.022808321107688722,"score_gpt":0.24945320494091985,"score_spread":0.22664488383323114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283024364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99662495,0.00019751301,0.00022341491,0.000035181954,0.0000019480926,0.00000685041,0.0019095801,0.000023904375,0.0009768083],"genre_scores_gemma":[0.9961404,0.00005838062,0.0004143993,0.000014633412,0.0000105507925,0.0000068090967,0.002925703,0.000008305995,0.00042080533],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995055,0.00008181378,0.000024112209,0.00014365464,0.00013958623,0.0001053386],"domain_scores_gemma":[0.99865794,0.00013675206,0.0005277242,0.00018737087,0.00020536003,0.00028486087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007212758,0.00020761449,0.0002457019,0.0026299437,0.00044935636,0.00065545423,0.0003356511,0.0001391837,0.0018207497],"category_scores_gemma":[0.0010767524,0.00014186325,0.0003553988,0.0019374774,0.00018707005,0.00044280544,0.0008228151,0.00016755893,0.00042534698],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041024035,0.000014876848,0.995248,0.000004690798,0.000058155187,0.000029284072,0.000050636718,0.0001651915,0.0009056288,0.000109218956,0.00037607213,0.0029972321],"study_design_scores_gemma":[0.000002872957,0.000007314208,0.99897575,0.0000012823735,0.000009096786,0.000027886092,0.000029172661,0.00031390795,0.00011874934,0.0000175702,0.00049434294,0.000001989736],"about_ca_topic_score_codex":0.036569517,"about_ca_topic_score_gemma":0.0603105,"teacher_disagreement_score":0.036569517,"about_ca_system_score_codex":0.00061311154,"about_ca_system_score_gemma":0.00046337416,"threshold_uncertainty_score":0.072713315},"labels":[],"label_agreement":null},{"id":"W4283164814","doi":"10.3847/1538-4357/ac6be9","title":"α-deep Probabilistic Inference (α-DPI): Efficient Uncertainty Quantification from Exoplanet Astrometry to Black Hole Feature Extraction","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Heising-Simons Foundation; National Science Foundation","keywords":"Physics; Astrometry; Exoplanet; Inference; Extraction (chemistry); Astronomy; Probabilistic logic; Astrophysics; Feature (linguistics); Artificial intelligence; Stars; Chromatography","score_opus":0.014084367967315123,"score_gpt":0.25356562381596903,"score_spread":0.2394812558486539,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283164814","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.015717683,0.00026351825,0.98230803,0.00029039526,0.000026923577,0.000027103448,0.00011737954,0.0005603973,0.0006887031],"genre_scores_gemma":[0.6650269,0.00042040567,0.33064932,0.00044495845,0.00013532484,0.00011280308,0.000773874,0.00022448089,0.0022120012],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992417,0.00023252012,0.000046989775,0.0002225124,0.0001798585,0.000076504104],"domain_scores_gemma":[0.99632865,0.0025225522,0.0003002798,0.00037882148,0.0003170831,0.00015257183],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028685152,0.00094467984,0.0012287439,0.00083000667,0.00051966636,0.0012540215,0.0024742691,0.0012581779,0.001826769],"category_scores_gemma":[0.011909555,0.0008629305,0.00089068786,0.00086200394,0.0013388889,0.0021473404,0.0030465268,0.0028047534,0.0002862596],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001332745,0.000064743406,0.0030023952,0.000110688095,0.00008926286,0.00013623037,0.00010803898,0.83452314,0.0020160426,0.032013442,0.0019552878,0.12584738],"study_design_scores_gemma":[0.0000047315484,0.0000056392523,0.00011492083,0.000004801304,0.0000033447966,0.000009779017,0.000003014993,0.9845276,0.00043266543,0.014692405,0.00019814639,0.0000030617714],"about_ca_topic_score_codex":0.006051361,"about_ca_topic_score_gemma":0.005660909,"teacher_disagreement_score":0.006051361,"about_ca_system_score_codex":0.0013856237,"about_ca_system_score_gemma":0.0017578454,"threshold_uncertainty_score":0.015170336},"labels":[],"label_agreement":null},{"id":"W4283168730","doi":"10.3847/1538-4357/ac6b9f","title":"Using the Sun to Measure the Primary Beam Response of the Canadian Hydrogen Intensity Mapping Experiment","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Okanagan University College; Perimeter Institute; University of British Columbia, Okanagan Campus; Herzberg Institute of Astrophysics; Thompson Rivers University; McGill University; University of British Columbia","funders":"National Research Council Canada; University of Toronto; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Canadian Institute for Advanced Research; Smithsonian Astrophysical Observatory; Western Canada Research Grid; Industry Canada; Canada Foundation for Innovation; National Science Foundation; Compute Canada; McGill University; Government of Canada","keywords":"Physics; Brightness; Sky; Beam (structure); Telescope; Intensity (physics); Calibration; Brightness temperature; Astronomy; Radio telescope; Astrophysics; Range (aeronautics); Optics; Remote sensing; Geography","score_opus":0.029544072079130183,"score_gpt":0.23350772986004964,"score_spread":0.20396365778091946,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283168730","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9396519,0.00024163445,0.0061528236,0.00023314588,0.0000637904,0.00016555915,0.013752301,0.00044309223,0.03929582],"genre_scores_gemma":[0.98387927,0.00012191591,0.0072216364,0.00014523035,0.000014465651,0.00006518455,0.0049458845,0.00007716798,0.003529315],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9992836,0.000031291464,0.0000073986125,0.0001340923,0.00039413047,0.00014945758],"domain_scores_gemma":[0.9987343,0.00006292621,0.00009016333,0.00013582951,0.0007564786,0.00022035702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005081429,0.00034877544,0.00027082366,0.00095934595,0.0015033503,0.0005695609,0.0006404222,0.00023000596,0.0024254518],"category_scores_gemma":[0.00081394735,0.00022323857,0.0001890035,0.0015841036,0.000441336,0.00022262789,0.0006492278,0.00044416226,0.0004093635],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018498739,0.00039125004,0.5637847,0.00020932501,0.00048332196,0.0003640999,0.001551893,0.0060143014,0.26716903,0.002910196,0.030387837,0.1248841],"study_design_scores_gemma":[0.000053944597,0.00007550964,0.94784784,0.000011070966,0.000041508032,0.000074890086,0.00025731727,0.002802499,0.03281626,0.00013735749,0.015836371,0.000045472672],"about_ca_topic_score_codex":0.7572188,"about_ca_topic_score_gemma":0.9161992,"teacher_disagreement_score":0.7572188,"about_ca_system_score_codex":0.0053699776,"about_ca_system_score_gemma":0.003955212,"threshold_uncertainty_score":0.48842198},"labels":[],"label_agreement":null},{"id":"W4283212094","doi":"10.3847/1538-4357/ac8102","title":"The Atari Disk, a Metal-poor Stellar Population in the Disk System of the Milky Way","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Population; Metallicity; Physics; Thin disk; Algorithm; Stars; Astrophysics; Computer science","score_opus":0.01003939109905481,"score_gpt":0.2133064298919124,"score_spread":0.2032670387928576,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283212094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99927706,0.00005088347,0.00033092152,0.000012588166,6.2619495e-7,0.0000034319182,0.000091813075,0.0000055682317,0.00022721593],"genre_scores_gemma":[0.9966757,0.000059787046,0.0021654726,0.000017466353,0.0000031445088,0.0000060616962,0.0004889412,0.000008970003,0.00057444687],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998796,0.000023636603,0.0000095601645,0.00004924943,0.0000208469,0.000017049371],"domain_scores_gemma":[0.9997347,0.000036662124,0.00007286192,0.00003648807,0.00004386396,0.000075521515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037086307,0.00018583747,0.0002019836,0.0009414694,0.00039080053,0.0006746667,0.0003027196,0.00017288729,0.0007105319],"category_scores_gemma":[0.0006821222,0.000117720796,0.00013239171,0.00062556606,0.00032828617,0.00041475255,0.0006587207,0.00012115529,0.00034585607],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000063565465,0.000018204415,0.97415257,0.00001714047,0.00002541039,0.00008492204,0.0005736971,0.0006777372,0.008472304,0.00025157537,0.00015081537,0.015512013],"study_design_scores_gemma":[0.0000123108675,0.00006520521,0.9931797,0.0000084315725,0.000022056756,0.0001252632,0.00043479286,0.0024206734,0.0019019508,0.00034515408,0.0014789774,0.000005520498],"about_ca_topic_score_codex":0.006924036,"about_ca_topic_score_gemma":0.011367774,"teacher_disagreement_score":0.006924036,"about_ca_system_score_codex":0.0003376197,"about_ca_system_score_gemma":0.00028079585,"threshold_uncertainty_score":0.013767481},"labels":[],"label_agreement":null},{"id":"W4283359361","doi":"10.3847/1538-4357/ac7b25","title":"1RXH J082623.6–505741: A New Long-period Cataclysmic Variable with an Evolved Donor and a Low Mass-transfer Rate","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Aeronautics and Space Administration","keywords":"Astrophysics; Orbital period; Physics; White dwarf; Cataclysmic variable star; Photometry (optics); Roche lobe; Light curve; Dwarf nova; Astronomy; Low Mass; Intermediate polar; Accretion (finance); Stars","score_opus":0.00829412916180971,"score_gpt":0.20327881957149735,"score_spread":0.19498469040968763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283359361","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99361104,0.00044669292,0.0003971738,0.00036296816,0.000090392714,0.000013963994,0.0003821456,0.00006861844,0.00462707],"genre_scores_gemma":[0.9971367,0.000056999703,0.0003325656,0.00020033018,0.00009888372,0.0000061853148,0.0005361348,0.000017415121,0.0016148152],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998568,0.000011261836,0.0000073105216,0.000060267823,0.000030422158,0.000033950735],"domain_scores_gemma":[0.99973136,0.0000134511265,0.00006685366,0.000028657094,0.00002424706,0.00013550803],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002898291,0.0004803007,0.00041492973,0.0006057953,0.0011314298,0.0009558043,0.000519006,0.000653472,0.0028906227],"category_scores_gemma":[0.00025064588,0.00013671593,0.00015989928,0.0004666521,0.00058026944,0.00037558159,0.00046207823,0.00052102236,0.0014027682],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009374878,0.00081870187,0.73801196,0.00014999033,0.00016303669,0.04405435,0.0012752182,0.0010209093,0.13779561,0.0072180945,0.022939352,0.04561523],"study_design_scores_gemma":[0.0001641137,0.0006405183,0.88706654,0.000053452604,0.00007613516,0.046987083,0.00079581403,0.0022187966,0.008077663,0.002546894,0.051309988,0.00006290878],"about_ca_topic_score_codex":0.0012221728,"about_ca_topic_score_gemma":0.001998192,"teacher_disagreement_score":0.0028906227,"about_ca_system_score_codex":0.0005068011,"about_ca_system_score_gemma":0.00016215231,"threshold_uncertainty_score":0.009670079},"labels":[],"label_agreement":null},{"id":"W4283456198","doi":"10.3847/1538-4357/ac7568","title":"The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). II. The Spatially Resolved Recent Star Formation History of M33","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Aeronautics and Space Administration","keywords":"Physics; Andromeda; Astrophysics; Panchromatic film; Galaxy; Spiral galaxy; Star formation; Advanced Camera for Surveys; Astronomy; Local Group; Measure (data warehouse); Milky Way","score_opus":0.013729565364309282,"score_gpt":0.20252320244577432,"score_spread":0.18879363708146504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283456198","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9835903,0.0002591998,0.0028950954,0.000062029576,0.000009002972,0.000046511068,0.008429139,0.00024909986,0.004459554],"genre_scores_gemma":[0.9831217,0.0001267342,0.008158307,0.00003607277,0.000020182493,0.000040324798,0.0071533504,0.00006996018,0.0012733705],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979895,0.00003101843,0.0000042698634,0.000066699096,0.00004672655,0.000052291947],"domain_scores_gemma":[0.999461,0.000044271863,0.00023488775,0.00012278697,0.000051047562,0.00008613097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025307288,0.0003084836,0.00019072622,0.0008456325,0.00018522945,0.00028824236,0.00036101742,0.00022326435,0.0016312957],"category_scores_gemma":[0.00070803496,0.00018743196,0.0003814393,0.00090732274,0.00012827151,0.00031951445,0.00041315146,0.00024827602,0.0005991834],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003499144,0.000070095346,0.8795745,0.000105447994,0.00029151022,0.0004508779,0.0004194468,0.005458389,0.040121727,0.0007952599,0.0070494744,0.06531343],"study_design_scores_gemma":[0.0000067271617,0.000025556315,0.99338245,0.000005693587,0.00001381902,0.00013659801,0.00003191768,0.002410258,0.0011208467,0.000042156338,0.0028136692,0.000010364329],"about_ca_topic_score_codex":0.023858942,"about_ca_topic_score_gemma":0.04887494,"teacher_disagreement_score":0.023858942,"about_ca_system_score_codex":0.00029562126,"about_ca_system_score_gemma":0.00015103388,"threshold_uncertainty_score":0.04744011},"labels":[],"label_agreement":null},{"id":"W4283653990","doi":"10.3847/1538-4357/ac79b2","title":"The Properties of Fast Yellow Pulsating Supergiants: FYPS Point the Way to Missing Red Supergiants","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; European Space Agency; Research Corporation for Scientific Advancement; Space Telescope Science Institute; University of Washington; Washington Research Foundation; Research Corporation for Science Advancement; National Science Foundation","keywords":"Supergiant; Physics; Red supergiant; Astrophysics; Stars; Supernova; Hertzsprung–Russell diagram; Astronomy; Luminosity; Stellar evolution; Large Magellanic Cloud; Blue supergiant; Galaxy","score_opus":0.02097728557231546,"score_gpt":0.2345649694827099,"score_spread":0.21358768391039445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283653990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99616784,0.00022319578,0.00047303137,0.000051016475,0.0000029938728,0.000004360465,0.0008834832,0.000044043336,0.002150023],"genre_scores_gemma":[0.9983693,0.000077548604,0.00022683876,0.000012177561,0.000007298274,0.0000021982926,0.0008488411,0.000015628142,0.00044019832],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999262,0.000005620168,0.0000047501826,0.000021254295,0.000018589719,0.000023500548],"domain_scores_gemma":[0.9995228,0.0000785721,0.00015558761,0.00006595487,0.000051300205,0.0001257346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021710474,0.00019032239,0.00021911779,0.0012969953,0.0002961081,0.0006153704,0.00015072498,0.0001505638,0.0030362238],"category_scores_gemma":[0.0006513573,0.000086609754,0.00016017898,0.0010559447,0.00028855086,0.00047441002,0.00042399528,0.0002534493,0.00079650903],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019741246,0.000019690768,0.96010804,0.000039631424,0.00003584402,0.00020380667,0.00032648613,0.000488004,0.0129225105,0.0005676342,0.0012719665,0.023818918],"study_design_scores_gemma":[0.0000024639817,0.000016351421,0.997509,0.0000027437077,0.000003678749,0.00016058747,0.00009416973,0.00024578985,0.0005773405,0.00021990878,0.0011663478,0.0000016667398],"about_ca_topic_score_codex":0.0021673269,"about_ca_topic_score_gemma":0.0019045596,"teacher_disagreement_score":0.0030362238,"about_ca_system_score_codex":0.0001505087,"about_ca_system_score_gemma":0.000075789685,"threshold_uncertainty_score":0.0101572275},"labels":[],"label_agreement":null},{"id":"W4283687295","doi":"10.3847/1538-4357/ac7b86","title":"Universal Relations for the Increase in the Mass and Radius of a Rotating Neutron Star","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Physics; RADIUS; Equation of state; Hydrostatic equilibrium; Astrophysics; Quantum mechanics","score_opus":0.011438534367820054,"score_gpt":0.28786730169470676,"score_spread":0.2764287673268867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283687295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93999577,0.00017248816,0.05803921,0.00009611313,0.000020540469,0.000028436847,0.00020481442,0.0005169946,0.00092562265],"genre_scores_gemma":[0.98227227,0.000030193,0.017333463,0.000008431545,0.000004914537,0.000013164042,0.00019330328,0.00005535127,0.00008886055],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9993261,0.00014361064,0.00004740367,0.00027842488,0.00013541125,0.00006897207],"domain_scores_gemma":[0.9915623,0.0051721516,0.001259009,0.0012481456,0.0005146232,0.0002437195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020133848,0.00030485154,0.00033658807,0.0013620185,0.00035171176,0.00051611435,0.00075810816,0.00048588956,0.0008973222],"category_scores_gemma":[0.021204809,0.00025468448,0.00042523773,0.0006480372,0.0010894628,0.00081284903,0.00065049436,0.0006103733,0.000103111066],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013986768,0.0000770662,0.12412913,0.00007547333,0.000087720575,0.0001143321,0.00020140794,0.8205166,0.0081103295,0.018336233,0.00040103408,0.027810775],"study_design_scores_gemma":[0.00001668625,0.000031795418,0.017858576,0.000013179105,0.000011337882,0.000094595816,0.000028223312,0.9707092,0.004238656,0.0065999175,0.0003788942,0.000018822613],"about_ca_topic_score_codex":0.003691092,"about_ca_topic_score_gemma":0.0029212087,"teacher_disagreement_score":0.003691092,"about_ca_system_score_codex":0.00085131574,"about_ca_system_score_gemma":0.0005676159,"threshold_uncertainty_score":0.010647953},"labels":[],"label_agreement":null},{"id":"W4283711301","doi":"10.3847/1538-4357/ac6e68","title":"VERTICO II: How H i-identified Environmental Mechanisms Affect the Molecular Gas in Cluster Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Royal Military College of Canada; McMaster University; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Australian Research Council; National Research Foundation of Korea; Agencia Nacional de Investigación y Desarrollo; Canada Research Chairs; Science and Technology Facilities Council; National Research Foundation; Associated Universities; National Natural Science Foundation of China; Simons Foundation; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Cluster (spacecraft); Galaxy cluster; Astronomy; Brightest cluster galaxy; Galaxy; Affect (linguistics); Galaxy groups and clusters","score_opus":0.005592480125632683,"score_gpt":0.19800404593664353,"score_spread":0.19241156581101085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283711301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9531594,0.0034929963,0.003237158,0.0019052426,0.00013414896,0.00001571511,0.00031910167,0.00009985784,0.03763634],"genre_scores_gemma":[0.99662554,0.000729373,0.00045847168,0.00017799143,0.0001090222,0.000006405953,0.00013858138,0.000045053483,0.0017095888],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997842,0.000052709536,0.000005036791,0.000075702934,0.00003720368,0.000045226578],"domain_scores_gemma":[0.999647,0.00014085695,0.000060584367,0.00006590321,0.000035745015,0.00004997288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036660652,0.0001695048,0.00021070498,0.0003748464,0.00039011508,0.0020653491,0.00041882362,0.0004209631,0.0020643529],"category_scores_gemma":[0.0012027095,0.00015539715,0.0002078835,0.00051553664,0.000792947,0.0009222913,0.0008570428,0.0005327917,0.000237764],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010184341,0.00017868528,0.5946565,0.0005517571,0.0004666192,0.0029823473,0.0048895706,0.027198145,0.09390601,0.10496657,0.0140601555,0.15512514],"study_design_scores_gemma":[0.00004900097,0.00018772656,0.89828753,0.00007640894,0.000099767014,0.00044174833,0.0018882263,0.018201709,0.0108803585,0.03307167,0.036731347,0.000084449886],"about_ca_topic_score_codex":0.0038807401,"about_ca_topic_score_gemma":0.0041194726,"teacher_disagreement_score":0.0038807401,"about_ca_system_score_codex":0.00070161885,"about_ca_system_score_gemma":0.00019768746,"threshold_uncertainty_score":0.007716298},"labels":[],"label_agreement":null},{"id":"W4283729268","doi":"10.3847/1538-4357/ac7c10","title":"Investigating the Origin of X-Ray Jets: A Case Study of Four Hybrid Morphology MOJAVE Blazars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Blazar; Physics; Astrophysics; Jet (fluid); Synchrotron; Spectral energy distribution; Astronomy; Galaxy; Gamma ray; Optics","score_opus":0.02297065553134292,"score_gpt":0.25187769033852764,"score_spread":0.22890703480718472,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283729268","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99941313,0.000042285614,0.00014452489,0.0000098349765,6.1750745e-7,0.0000047554486,0.00002018422,0.0000059048225,0.0003588155],"genre_scores_gemma":[0.99915445,0.00003146987,0.0006057257,0.000007976712,0.0000025398203,0.0000017181908,0.000052926098,0.000003685365,0.00013951884],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998342,0.000033043838,0.000010069624,0.00004309346,0.000035469086,0.00004408738],"domain_scores_gemma":[0.99955875,0.00013664899,0.00014799816,0.00004544486,0.000034895857,0.0000762586],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028542566,0.0003178765,0.00025838107,0.0011992508,0.00080566586,0.0010253008,0.00036028493,0.00046291586,0.0005358602],"category_scores_gemma":[0.00054302334,0.0001928469,0.000346128,0.00069602765,0.0005175361,0.0002466116,0.0004596134,0.0002566553,0.000100475234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035689646,0.00016368639,0.95697594,0.00003788009,0.000109943416,0.0137101505,0.002618891,0.0012506697,0.0152735915,0.00084068824,0.00014940859,0.0085121235],"study_design_scores_gemma":[0.000031828964,0.00019284696,0.9845116,0.000014847662,0.00005904959,0.0065948567,0.0018874409,0.0026318717,0.0024002588,0.00019003576,0.0014673368,0.00001790883],"about_ca_topic_score_codex":0.0070660664,"about_ca_topic_score_gemma":0.010903819,"teacher_disagreement_score":0.0070660664,"about_ca_system_score_codex":0.0003465259,"about_ca_system_score_gemma":0.000121800025,"threshold_uncertainty_score":0.014049888},"labels":[],"label_agreement":null},{"id":"W4283734119","doi":"10.3847/1538-4357/ac7c6d","title":"Young, Blue, and Isolated Stellar Systems in the Virgo Cluster. I. 2D Optical Spectroscopy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Virgo Cluster; Physics; Astrophysics; Galaxy; Hubble space telescope; Cluster (spacecraft); Metallicity; Astronomy; Spectroscopy; Star formation; Galaxy cluster; Computer science","score_opus":0.005436936298848955,"score_gpt":0.20837983905169144,"score_spread":0.2029429027528425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283734119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991474,0.00020260044,0.00008811895,0.000009934933,7.14439e-7,0.0000030578656,0.000058694837,0.000004311138,0.00048515876],"genre_scores_gemma":[0.9994931,0.00004888111,0.00021377571,0.000007681923,0.0000019136085,0.0000018901225,0.00012980057,0.000001528264,0.00010144612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990094,0.00001583481,0.000003818814,0.000033278462,0.000018160621,0.00002796438],"domain_scores_gemma":[0.9996499,0.000058169306,0.000112383445,0.000027850276,0.000024446637,0.00012732502],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028898835,0.00019264015,0.00018903938,0.0019655714,0.0004592216,0.0006493856,0.00028860397,0.00023744798,0.00061046693],"category_scores_gemma":[0.0004243477,0.00014452696,0.00013490654,0.0006636306,0.00043817025,0.00028589304,0.00071116834,0.00019111013,0.000115794064],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038108006,0.000053444943,0.95816094,0.000034086752,0.000046567122,0.00027616133,0.00059684954,0.0012869962,0.03136993,0.0007752613,0.0001471337,0.006871593],"study_design_scores_gemma":[0.0000053021054,0.00004928741,0.99684554,0.000005261491,0.000013342274,0.0001620985,0.00025065016,0.0013121635,0.0008533824,0.0001826831,0.00031445557,0.0000058316873],"about_ca_topic_score_codex":0.0058738193,"about_ca_topic_score_gemma":0.010547104,"teacher_disagreement_score":0.0058738193,"about_ca_system_score_codex":0.00045730133,"about_ca_system_score_gemma":0.0001549565,"threshold_uncertainty_score":0.011679292},"labels":[],"label_agreement":null},{"id":"W4283743339","doi":"10.3847/1538-4357/ac7c74","title":"The Astropy Project: Sustaining and Growing a Community-oriented Open-source Project and the Latest Major Release (v5.0) of the Core Package*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Waypoint Centre for Mental Health Care; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Horizon 2020 Framework Programme; Agencia Nacional de Investigación y Desarrollo; Instituto de Astrofísica de Andalucía; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Magyar Tudományos Akadémia; Macquarie University; Stellar Astrophysics Centre; Ministerio de Ciencia, Innovación y Universidades; Gordon and Betty Moore Foundation; Danmarks Grundforskningsfond; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Science and Technology Facilities Council; National Research Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Interoperability; Python (programming language); Open source; Key (lock); Computer science; Systems engineering; Core (optical fiber); Software engineering; Engineering management; World Wide Web; Engineering; Telecommunications; Computer security; Operating system; Software","score_opus":0.02034964739329553,"score_gpt":0.29044198231640805,"score_spread":0.2700923349231125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283743339","genre_codex":"methods","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.013785301,0.0030041398,0.5612778,0.020966912,0.006229883,0.0016531635,0.03284211,0.3214996,0.038741075],"genre_scores_gemma":[0.027192034,0.0019003304,0.6060095,0.004627932,0.0019459382,0.0024300565,0.11381268,0.21397838,0.028103204],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9891585,0.002468172,0.00065269356,0.0013918785,0.0050357576,0.001293049],"domain_scores_gemma":[0.9469896,0.008584407,0.0026639898,0.009580171,0.016604569,0.015577336],"candidate_categories":["open_science"],"consensus_categories":[],"category_scores_codex":[0.024702836,0.0023015046,0.0015856307,0.0041630166,0.0037883036,0.009233248,0.006053518,0.0024420843,0.027130842],"category_scores_gemma":[0.052463405,0.001728923,0.0022985975,0.0041039265,0.0028466203,0.012005812,0.018832548,0.009011426,0.04375843],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005051517,0.0003150877,0.004004291,0.001023985,0.00014572308,0.00024445486,0.0012973128,0.0014067822,0.007456462,0.025290972,0.7207896,0.23752019],"study_design_scores_gemma":[0.00016466304,0.0001553722,0.0036636242,0.00048084735,0.00006517051,0.0002632581,0.00018664516,0.0044429977,0.004531256,0.021113344,0.9647253,0.00020753595],"about_ca_topic_score_codex":0.005543712,"about_ca_topic_score_gemma":0.003476623,"teacher_disagreement_score":0.9939465,"about_ca_system_score_codex":0.0015417704,"about_ca_system_score_gemma":0.016662868,"threshold_uncertainty_score":0.13064265},"labels":[],"label_agreement":null},{"id":"W4283761183","doi":"10.3847/1538-4357/ac88d0","title":"A Mildly Relativistic Outflow Launched Two Years after Disruption in Tidal Disruption Event AT2018hyz","year":2022,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Outflow; Physics; Astrophysics; RADIUS; Kinetic energy; Approx; Light curve; Jet (fluid); Meteorology; Mechanics","score_opus":0.012038310779113466,"score_gpt":0.2693545481392339,"score_spread":0.2573162373601204,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283761183","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99875426,0.000048227455,0.00021495234,0.000061334715,0.0000107595115,0.0000049731393,0.00023092622,0.000027751172,0.00064691313],"genre_scores_gemma":[0.99908113,0.000022436348,0.00012724737,0.000024869043,0.000014354346,0.00000282957,0.00046735795,0.0000034041113,0.0002563537],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999168,0.0000044683115,0.0000038534577,0.000015364694,0.000019833433,0.000039811846],"domain_scores_gemma":[0.99977726,0.000020504382,0.000072922434,0.000019369663,0.000022629301,0.00008723621],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015251827,0.00018712622,0.00025973312,0.00056277966,0.0005854311,0.0005132855,0.00021072669,0.00041252963,0.00074890605],"category_scores_gemma":[0.00025966973,0.000091265254,0.00026403563,0.00034507073,0.0002839811,0.00019215274,0.00070660556,0.0003565761,0.00016109941],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008358953,0.00015584184,0.9124953,0.0000600282,0.0000980955,0.01102584,0.0011931807,0.0015372987,0.055582203,0.0009302955,0.00119401,0.014891913],"study_design_scores_gemma":[0.000010277956,0.00007939678,0.9945246,0.0000060749167,0.000015585267,0.00057448103,0.0002316276,0.0009711491,0.0020115655,0.00009972711,0.0014680796,0.000007487512],"about_ca_topic_score_codex":0.0077611534,"about_ca_topic_score_gemma":0.008612746,"teacher_disagreement_score":0.0077611534,"about_ca_system_score_codex":0.00064139685,"about_ca_system_score_gemma":0.00018978237,"threshold_uncertainty_score":0.015431941},"labels":[],"label_agreement":null},{"id":"W4283811053","doi":"10.3847/1538-4357/ac7c05","title":"Hard X-Ray Emission from the Eastern Jet of SS 433 Powering the W50 “Manatee” Nebula: Evidence for Particle Reacceleration","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Particle acceleration; Nebula; Pulsar wind nebula; Vela; Supernova remnant; Pulsar; Spectral index; Jet (fluid); Acceleration; Crab Nebula; Astronomy; Supernova; Stars; Spectral line","score_opus":0.03968611255171488,"score_gpt":0.27001102990108783,"score_spread":0.23032491734937294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4283811053","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988953,0.000053050717,0.00015423459,0.00000846279,0.0000010351472,0.000002881308,0.000047926776,0.00001279437,0.00082426454],"genre_scores_gemma":[0.99952495,0.000026974674,0.00018539892,0.000012778113,0.0000021947442,0.0000014501104,0.000082981656,0.0000040807354,0.00015926393],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999567,0.0000032363848,0.0000032626363,0.000011829063,0.000012640303,0.000012392188],"domain_scores_gemma":[0.99983394,0.00002027465,0.000060442748,0.000019972622,0.000021782684,0.00004348698],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011894348,0.00018184414,0.00015983921,0.00050964206,0.00022702734,0.00050754944,0.00020814271,0.00018881545,0.0014082594],"category_scores_gemma":[0.0001673263,0.00016757697,0.00016899193,0.00031843278,0.0002528399,0.00016950836,0.00039364534,0.00014684502,0.00026687834],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033234773,0.00008276253,0.74720836,0.00004545994,0.00009218645,0.00279928,0.0005013998,0.0003665401,0.23989469,0.00029491252,0.00021245946,0.008169639],"study_design_scores_gemma":[0.000005315194,0.000064474225,0.99425864,0.0000040947643,0.00001416562,0.0006525962,0.00012383875,0.00040303354,0.0039593717,0.000051632192,0.00045856976,0.0000041535427],"about_ca_topic_score_codex":0.002749436,"about_ca_topic_score_gemma":0.0047179507,"teacher_disagreement_score":0.002749436,"about_ca_system_score_codex":0.00014324416,"about_ca_system_score_gemma":0.00007674372,"threshold_uncertainty_score":0.0054668784},"labels":[],"label_agreement":null},{"id":"W4284664269","doi":"10.3847/1538-4357/ac7c0f","title":"Synthetic Polarization Maps of an Outflow Zone from Magnetohydrodynamic Simulations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Royal Bank of Canada","funders":"","keywords":"Physics; Polarization (electrochemistry); Magnetohydrodynamics; Magnetic field; Astrophysics; Magnetohydrodynamic drive; Outflow; Radiative transfer; Toroid; Field line; Sky; Perpendicular; Computational physics; Optics; Plasma; Geometry","score_opus":0.006296417235603631,"score_gpt":0.21833005260213975,"score_spread":0.21203363536653613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4284664269","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9857964,0.00005794865,0.008217072,0.00018481477,0.00003578802,0.000039431376,0.0015781721,0.0004181405,0.0036723008],"genre_scores_gemma":[0.9956982,0.000027707396,0.0029204246,0.000021737871,0.00001108254,0.000023040797,0.0010772081,0.000041366264,0.00017934122],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998889,0.00003565104,0.000004344577,0.00001791659,0.00002442051,0.000028834276],"domain_scores_gemma":[0.9993469,0.00034737785,0.000056768957,0.000061539904,0.00009844784,0.00008893266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029822957,0.00044108325,0.0003304415,0.00055227045,0.0003524084,0.0006418056,0.0006236858,0.00072878523,0.0012014174],"category_scores_gemma":[0.0013993025,0.00022348687,0.00053823466,0.000579833,0.00046700097,0.00026824002,0.0004119076,0.0005014421,0.000116000054],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019503883,0.00013049298,0.0075177145,0.000035107907,0.00006481561,0.00018839039,0.00007227512,0.9842466,0.003752736,0.0011746933,0.000651193,0.001970899],"study_design_scores_gemma":[0.00007156099,0.00003226405,0.0038694474,0.0000050037993,0.000008729127,0.000024005685,0.00003340286,0.99380386,0.0011267534,0.00066636567,0.00034670255,0.000011869767],"about_ca_topic_score_codex":0.004764902,"about_ca_topic_score_gemma":0.0021163628,"teacher_disagreement_score":0.004764902,"about_ca_system_score_codex":0.00042542102,"about_ca_system_score_gemma":0.0003321809,"threshold_uncertainty_score":0.009474337},"labels":[],"label_agreement":null},{"id":"W4284688645","doi":"10.3847/1538-4357/ac714a","title":"The Host Galaxy and Rapidly Evolving Broad-line Region in the Changing-look Active Galactic Nucleus 1ES 1927+654","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"National Key Research and Development Program of China; Key Programme; European Research Council; Israel Science Foundation","keywords":"Physics; Balmer series; Astrophysics; Galaxy; Active galactic nucleus; Emission spectrum; Line (geometry); Astronomy; Spectroscopy; Spectral line; Accretion (finance)","score_opus":0.01316061046981075,"score_gpt":0.23035139344354771,"score_spread":0.21719078297373695,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4284688645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991726,0.000033808545,0.000049066653,0.000012863804,0.0000013125872,0.000001553678,0.000082653045,0.000006528565,0.0006395469],"genre_scores_gemma":[0.99936837,0.000017379303,0.00008890006,0.0000110018755,0.000002451902,0.0000012246581,0.00022846505,0.0000030919427,0.0002791753],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996734,0.0000037740092,0.000001231423,0.000010299315,0.000006667061,0.000010755858],"domain_scores_gemma":[0.9998084,0.000023433173,0.00007666723,0.000011795362,0.00002220778,0.00005760963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008150572,0.000105625695,0.00008970534,0.0004426959,0.00017847677,0.0002889145,0.00017559767,0.00015407031,0.0015056402],"category_scores_gemma":[0.0002493454,0.00007907543,0.000082964674,0.0001792466,0.00014664549,0.00016948475,0.00023234056,0.00014092932,0.00030667346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016448282,0.00007034744,0.9494721,0.000010431763,0.000023443772,0.0009112849,0.00021776078,0.00023906332,0.04227351,0.00013363166,0.000390329,0.006093516],"study_design_scores_gemma":[0.0000023804362,0.00002766683,0.998247,0.0000014548638,0.0000059554204,0.00025109568,0.00009944859,0.00027583833,0.0007802464,0.00002736733,0.0002795709,0.0000018883708],"about_ca_topic_score_codex":0.007483612,"about_ca_topic_score_gemma":0.010513881,"teacher_disagreement_score":0.007483612,"about_ca_system_score_codex":0.00025062368,"about_ca_system_score_gemma":0.0000444004,"threshold_uncertainty_score":0.014880061},"labels":[],"label_agreement":null},{"id":"W4284969413","doi":"10.3847/1538-4357/ac69ce","title":"NICER X-Ray Observations of Eta Carinae during Its Most Recent Periastron Passage","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Ejecta; Flux (metallurgy); X-ray; Shock (circulatory); Bow shock (aerodynamics); Astronomy; Shock wave; Optics","score_opus":0.023273353106021837,"score_gpt":0.23294467769568178,"score_spread":0.20967132458965995,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4284969413","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99613404,0.00022913296,0.00013650196,0.00003383823,0.0000055941146,0.0000074786312,0.00063176977,0.000041709907,0.0027799103],"genre_scores_gemma":[0.9971951,0.0000716025,0.0004889919,0.000028436807,0.000019012115,0.000008036329,0.0015479635,0.00001313742,0.0006277147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998167,0.000021651396,0.000009643973,0.000053800944,0.00006087963,0.00003727646],"domain_scores_gemma":[0.99949694,0.000043481192,0.00016602302,0.0000823716,0.00009327766,0.00011798556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038051972,0.00018175642,0.0003279718,0.00074684946,0.0006067244,0.00046323304,0.00034118426,0.00040882846,0.000745361],"category_scores_gemma":[0.0004654892,0.00021309571,0.00028092385,0.00033271592,0.00019719612,0.0003059603,0.0006239997,0.0002902538,0.00041157453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00097614323,0.00011628731,0.8324666,0.000109788365,0.00017309401,0.0011134231,0.00092510827,0.0008364566,0.14681695,0.00018011653,0.0016826496,0.014603381],"study_design_scores_gemma":[0.0000052202854,0.000059009144,0.99748516,0.000004682746,0.00000993372,0.00020387715,0.000039493774,0.00021390915,0.00077614083,0.0000072062335,0.0011908398,0.000004430331],"about_ca_topic_score_codex":0.003135475,"about_ca_topic_score_gemma":0.009863803,"teacher_disagreement_score":0.003135475,"about_ca_system_score_codex":0.00026047733,"about_ca_system_score_gemma":0.000106692765,"threshold_uncertainty_score":0.006234467},"labels":[],"label_agreement":null},{"id":"W4284972696","doi":"10.3847/1538-4357/ac82b0","title":"Recovering the Star Formation Histories of Recently Quenched Galaxies: The Impact of Model and Prior Choices","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Galaxy; Astrophysics; Star formation; Star (game theory); Galaxy formation and evolution; Astronomy","score_opus":0.015972997004419915,"score_gpt":0.24127472508166556,"score_spread":0.22530172807724563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4284972696","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.948683,0.00019413262,0.048623867,0.00039488776,0.000016780847,0.000026912381,0.0007455637,0.0004429426,0.0008719059],"genre_scores_gemma":[0.99168795,0.00004589221,0.007057303,0.00008131606,0.000009924346,0.0000140540205,0.0007931883,0.000074253156,0.0002360985],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.998868,0.0006285555,0.000044750588,0.00026172047,0.00010325929,0.000093697054],"domain_scores_gemma":[0.9847115,0.011137011,0.0008379922,0.0022702476,0.0005086442,0.00053447555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007534615,0.00058207527,0.0007180886,0.0006644397,0.0005702774,0.0013433485,0.0018155695,0.0010676297,0.0013217856],"category_scores_gemma":[0.021980982,0.00045708058,0.0011018105,0.00050890876,0.0011812032,0.0019883607,0.0009314274,0.0014578563,0.0002550874],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032418876,0.00009855943,0.084627844,0.000053844018,0.00019856176,0.00012660462,0.00014569919,0.8951836,0.0022341746,0.0051812357,0.0007507039,0.011075086],"study_design_scores_gemma":[0.000031074585,0.00008000644,0.020756299,0.000028686936,0.00003760961,0.00008467869,0.00006894658,0.97051114,0.0018003965,0.005955965,0.00059578364,0.000049457503],"about_ca_topic_score_codex":0.020746764,"about_ca_topic_score_gemma":0.013506686,"teacher_disagreement_score":0.020746764,"about_ca_system_score_codex":0.0013551216,"about_ca_system_score_gemma":0.00078958075,"threshold_uncertainty_score":0.041252017},"labels":[],"label_agreement":null},{"id":"W4285045546","doi":"10.3847/1538-4357/ac7466","title":"Deep Very Long Baseline Interferometry Observations Challenge Previous Evidence of a Binary Supermassive Black Hole Residing in Seyfert Galaxy NGC 7674","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Supermassive black hole; Very-long-baseline interferometry; Physics; Astrophysics; Very Long Baseline Array; Galaxy; Active galactic nucleus; Binary black hole; Binary number; Astronomy; Gravitational wave","score_opus":0.03230745182238893,"score_gpt":0.2605521246293631,"score_spread":0.2282446728069742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285045546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99807703,0.00017157554,0.0002594395,0.0001020174,0.0000060716784,0.0000012932157,0.000035505418,0.00001158025,0.0013354031],"genre_scores_gemma":[0.99944454,0.00005425827,0.00023285828,0.000031653395,0.000017272465,7.999398e-7,0.000063145475,0.0000013704534,0.00015420142],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998161,0.000015814589,0.000008533673,0.000030708296,0.000054616004,0.000074263815],"domain_scores_gemma":[0.9992213,0.00015363596,0.00030407388,0.0001101727,0.000083036706,0.00012775845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003099133,0.00017900184,0.00020024015,0.0010066931,0.0005572973,0.0007383824,0.00032983688,0.0003765361,0.0016378531],"category_scores_gemma":[0.0008520416,0.000097313605,0.00010551002,0.0005019643,0.00080011715,0.0006334106,0.0006383312,0.00027852578,0.00030162575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014963277,0.00006994112,0.8998846,0.000052465868,0.00007328662,0.0015799286,0.00076663366,0.00062998326,0.07430649,0.0024328285,0.0009885323,0.019065779],"study_design_scores_gemma":[0.000005290641,0.00003816905,0.9938652,0.000011094172,0.000021041677,0.0004396995,0.0006932882,0.0005050687,0.002225718,0.0006252481,0.0015640142,0.000006085647],"about_ca_topic_score_codex":0.0042952825,"about_ca_topic_score_gemma":0.011317162,"teacher_disagreement_score":0.0042952825,"about_ca_system_score_codex":0.00048228327,"about_ca_system_score_gemma":0.00017142436,"threshold_uncertainty_score":0.008540571},"labels":[],"label_agreement":null},{"id":"W4285046073","doi":"10.3847/1538-4357/ac746b","title":"Probing Population III Initial Mass Functions with He ii/Hα Intensity Mapping","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Astrophysics; Stars; Population; Star formation; Redshift; Galaxy; Intensity mapping; Initial mass function; Line (geometry); H-alpha; Spectral line; Emission spectrum; Astronomy","score_opus":0.01142381324679532,"score_gpt":0.2053424778580698,"score_spread":0.1939186646112745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285046073","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9823282,0.000058565813,0.015414646,0.00001452434,0.0000023511193,0.0000062323275,0.00037012898,0.00025381063,0.0015515733],"genre_scores_gemma":[0.9946637,0.000015523774,0.004902975,0.000006582458,0.0000022339987,0.0000041639228,0.00021222503,0.000017644,0.00017483847],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992526,0.000015097215,0.0000025019601,0.000024931438,0.000015044854,0.000017149301],"domain_scores_gemma":[0.9996383,0.00010817389,0.00010390727,0.000050759783,0.000044995555,0.0000537777],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028212712,0.00028071983,0.00011106333,0.0006690415,0.000109771216,0.00029145923,0.00023726694,0.00018996611,0.0011122746],"category_scores_gemma":[0.0006458594,0.000099477664,0.00016070371,0.0002996829,0.00010660123,0.00026861342,0.00032517905,0.00015048416,0.00026912277],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032426615,0.000073191564,0.80107886,0.0000379878,0.00010121524,0.00011997344,0.00011215757,0.01425823,0.1473082,0.0012420816,0.0003316823,0.03501221],"study_design_scores_gemma":[0.000010728306,0.00011566147,0.7828362,0.000010377981,0.000036092817,0.0001842763,0.000073992,0.12885413,0.08565383,0.0009657372,0.001235439,0.000023506525],"about_ca_topic_score_codex":0.0007388724,"about_ca_topic_score_gemma":0.0007742953,"teacher_disagreement_score":0.0011122746,"about_ca_system_score_codex":0.00015165123,"about_ca_system_score_gemma":0.00005008862,"threshold_uncertainty_score":0.0037209392},"labels":[],"label_agreement":null},{"id":"W4285098442","doi":"10.3847/1538-4357/ac63c7","title":"COMAP Early Science. V. Constraints and Forecasts at z ∼ 3","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Jet Propulsion Laboratory; Stanford Research Computing Center, Stanford University; Universitetet i Oslo; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; California Institute of Technology; European Commission; University of Miami; York University; Science and Technology Facilities Council; University of Toronto; Keck Institute for Space Studies; Norges Forskningsråd; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Pathfinder; Galaxy; Spectral density; Redshift; Intensity mapping; Astrophysics; Context (archaeology); Halo; Limit (mathematics); Statistics; Computer science; Mathematics; Geography; Mathematical analysis","score_opus":0.0083117778036286,"score_gpt":0.20940790209480836,"score_spread":0.20109612429117976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4285098442","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5442937,0.004980725,0.08013222,0.030132296,0.0005896706,0.00015671432,0.14032044,0.01780859,0.1815856],"genre_scores_gemma":[0.9290853,0.0013185954,0.024001598,0.0011357283,0.00025668475,0.00008680325,0.035955854,0.0010809491,0.0070784786],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99964464,0.000054495256,0.000011634266,0.00008173096,0.00014061839,0.000066892564],"domain_scores_gemma":[0.99702364,0.0006758788,0.00065974874,0.0003550426,0.0007039857,0.0005817176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013835357,0.00054831145,0.00038662305,0.0019058354,0.0005853552,0.0027619293,0.0010263382,0.0009566525,0.010488696],"category_scores_gemma":[0.0070574535,0.00034659164,0.00041441253,0.0015963742,0.00042616623,0.0019205677,0.0011106589,0.0012080306,0.0038427648],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082468905,0.00009812865,0.2633891,0.0004393487,0.0001293768,0.00067526347,0.000536081,0.17760332,0.0038884939,0.13947587,0.22889988,0.18404043],"study_design_scores_gemma":[0.00012300102,0.000082881714,0.16187891,0.0003228307,0.000056206827,0.00022730728,0.00043192974,0.37066898,0.0054106493,0.24022491,0.22039291,0.00017944671],"about_ca_topic_score_codex":0.037752986,"about_ca_topic_score_gemma":0.016537923,"teacher_disagreement_score":0.037752986,"about_ca_system_score_codex":0.0022660466,"about_ca_system_score_gemma":0.0014792539,"threshold_uncertainty_score":0.07506651},"labels":[],"label_agreement":null},{"id":"W4286592297","doi":"10.3847/1538-4357/ac76c0","title":"Evolution of a Relativistic Outflow and X-Ray Corona in the Extreme Changing-look AGN 1ES 1927+654","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"European Research Council; Israel Science Foundation; Nuclear Safety and Security Commission; Council for Higher Education; United States-Israel Binational Science Foundation; Canadian Institute for Advanced Research; Fondo Nacional de Desarrollo Científico y Tecnológico; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Accretion (finance); Outflow; Active galactic nucleus; Luminosity; Eddington luminosity; Flux (metallurgy); Spectral line; Black-body radiation; Astronomy; Emission spectrum; Galaxy; Radiation; Optics","score_opus":0.018348302506636858,"score_gpt":0.21903154618217546,"score_spread":0.2006832436755386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4286592297","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99845374,0.0000640301,0.00022415063,0.00007217095,0.000005523523,0.000003942559,0.0001304486,0.000033026798,0.0010130053],"genre_scores_gemma":[0.9988838,0.000025782756,0.00023129782,0.000021180605,0.00000774406,0.0000024494002,0.00027659396,0.000011279153,0.00053987396],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999453,0.0000070485644,0.0000023094794,0.00001844688,0.000013935091,0.000013013186],"domain_scores_gemma":[0.99986494,0.000013014771,0.000048237966,0.000009993018,0.000016152562,0.000047601065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016018907,0.00016052899,0.00019332024,0.0004973014,0.00033038793,0.00048698758,0.00028718822,0.00033877106,0.0010853668],"category_scores_gemma":[0.00026023109,0.00012629417,0.00021412465,0.0002409689,0.00019987962,0.00019128369,0.00044246283,0.00029596614,0.0002355397],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020180941,0.00016410697,0.94553715,0.000026663838,0.0000723104,0.003942079,0.00040727487,0.006551377,0.030444691,0.001051202,0.0018321734,0.009769169],"study_design_scores_gemma":[0.000017853705,0.00010988816,0.9790011,0.000009186164,0.000023706514,0.00089696795,0.00027128545,0.016255721,0.0010267902,0.00037223875,0.0019960774,0.000019215777],"about_ca_topic_score_codex":0.004925347,"about_ca_topic_score_gemma":0.005963677,"teacher_disagreement_score":0.004925347,"about_ca_system_score_codex":0.00045654282,"about_ca_system_score_gemma":0.00010655489,"threshold_uncertainty_score":0.009793341},"labels":[],"label_agreement":null},{"id":"W4286952808","doi":"10.3847/1538-4357/ac48f5","title":"Prospects for Measuring Off-axis Spins of Binary Black Holes with Plus-era Gravitational-wave Detectors","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"LIGO; Gravitational wave; Spins; Physics; Binary black hole; Spin (aerodynamics); Angular momentum; Precession; Astrophysics; Computational physics; Astronomy; Quantum mechanics; Condensed matter physics","score_opus":0.022403588798659325,"score_gpt":0.2841778597557869,"score_spread":0.2617742709571276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4286952808","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9832439,0.0001099118,0.014856211,0.00015063792,0.00001530328,0.000012997639,0.00009506923,0.00015455294,0.0013614648],"genre_scores_gemma":[0.9949468,0.0000134417605,0.004833071,0.000021505493,0.000004517484,0.000002934734,0.00007354861,0.000004376237,0.000099840545],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999524,0.00022451142,0.000014676426,0.0000918553,0.0000955545,0.000049472466],"domain_scores_gemma":[0.99818146,0.00090565823,0.00025887668,0.00023451414,0.0002755405,0.00014382422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0030113598,0.00039450923,0.00039179387,0.00035582494,0.000177255,0.00060985546,0.0005457451,0.00048832566,0.0006552394],"category_scores_gemma":[0.0041306303,0.00026889888,0.0001447083,0.00029697805,0.00052076316,0.001119775,0.00088743534,0.00031669013,0.0000757915],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025476702,0.0005347438,0.29980835,0.000111961366,0.00023743612,0.00019139852,0.00011890173,0.54943055,0.066462025,0.012620738,0.0013361465,0.06660011],"study_design_scores_gemma":[0.0001115692,0.0004515195,0.044635218,0.000012862316,0.000061204526,0.000111088026,0.000043989814,0.9132209,0.03523144,0.0046492955,0.0014314693,0.000039541723],"about_ca_topic_score_codex":0.0013990906,"about_ca_topic_score_gemma":0.0022809207,"teacher_disagreement_score":0.0030113598,"about_ca_system_score_codex":0.0004225439,"about_ca_system_score_gemma":0.00026543142,"threshold_uncertainty_score":0.015925765},"labels":[],"label_agreement":null},{"id":"W4287644149","doi":"10.3847/1538-4357/ac312a","title":"The Number Densities and Stellar Populations of Massive Galaxies at 3 &lt; z &lt; 6: A Diverse, Rapidly Forming Population in the Early Universe","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Astrophysics Division; Space Telescope Science Institute; Nuclear Safety and Security Commission; York University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Star formation; Redshift; Stellar mass; Population; Star (game theory); Cosmic time; Galaxy formation and evolution; Universe; Astronomy","score_opus":0.01029943576419548,"score_gpt":0.21334404866628218,"score_spread":0.2030446129020867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4287644149","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989544,0.000020294017,0.00006965748,0.000014764297,3.6011562e-7,0.0000016322999,0.0007187214,0.000008208037,0.00021195067],"genre_scores_gemma":[0.99829096,0.000032121003,0.00012424213,0.000008532635,0.0000025161323,0.0000023018094,0.0013038047,0.0000034156374,0.00023201815],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999014,0.000009526735,0.000005502074,0.000024097757,0.000024853289,0.00003459134],"domain_scores_gemma":[0.999215,0.00008646098,0.00028150072,0.000060948976,0.00009389458,0.00026219492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023917801,0.00012234876,0.00016672653,0.0011304935,0.0002286163,0.00068256987,0.00024226033,0.00018234279,0.0020682367],"category_scores_gemma":[0.000615091,0.000109373024,0.00026580773,0.00070315885,0.00024025222,0.00032135137,0.0004898326,0.00021572676,0.00062744995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000053072738,0.000014958649,0.9934916,0.0000050571966,0.000016492062,0.000033916214,0.00016694432,0.00025809737,0.0028427588,0.00013595511,0.00024462747,0.0027364246],"study_design_scores_gemma":[0.0000010548086,0.000007665225,0.999276,9.091457e-7,0.000002913642,0.000033481287,0.00004367195,0.0002840594,0.00019260828,0.00002444192,0.00013182453,0.0000013784561],"about_ca_topic_score_codex":0.006995334,"about_ca_topic_score_gemma":0.0090865055,"teacher_disagreement_score":0.006995334,"about_ca_system_score_codex":0.00019057479,"about_ca_system_score_gemma":0.00011488242,"threshold_uncertainty_score":0.013909221},"labels":[],"label_agreement":null},{"id":"W4288707872","doi":"10.3847/1538-4357/ac78e6","title":"On the H i Content of MaNGA Major Merger Pairs","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; Ministério da Ciência, Tecnologia e Inovação; Chinese Academy of Sciences; University of Oxford; York University; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Universities Space Research Association; Leibniz-Gemeinschaft; University of Notre Dame; Hebei Normal University; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; Natural Science Foundation of Hebei Province; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Galaxy; Astrophysics; Star formation; Sky; Galaxy formation and evolution; Content (measure theory); Galaxy merger; Mathematics","score_opus":0.014299912687835722,"score_gpt":0.20222001030669096,"score_spread":0.18792009761885523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4288707872","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953437,0.00006748008,0.000040896583,0.0000030339156,5.176349e-7,0.0000013756288,0.000119527416,0.0000031531308,0.00022969245],"genre_scores_gemma":[0.99964607,0.000018351395,0.000037055535,0.0000027892763,0.000001234818,0.000001364674,0.00021410143,0.000001245739,0.000077862445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998374,0.000024597917,0.0000113495325,0.00005632189,0.000025878202,0.00004451559],"domain_scores_gemma":[0.99960285,0.00004349783,0.00017158844,0.000036185498,0.000041214073,0.00010467816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017626364,0.00016530801,0.00023710748,0.0011472688,0.00036187147,0.00041229255,0.00018580223,0.00012436048,0.001254545],"category_scores_gemma":[0.0006010174,0.00009196591,0.00013640212,0.0005888085,0.0002953049,0.00022409523,0.0005092793,0.000093728915,0.0002816866],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012661779,0.000010453809,0.9866959,0.0000075693033,0.0000261728,0.00006331393,0.00014623388,0.00005887392,0.010759534,0.000050840754,0.000038818987,0.0020158137],"study_design_scores_gemma":[7.9392095e-7,0.000024614657,0.99907243,7.021076e-7,0.000005301154,0.000068207,0.000092361275,0.00008194603,0.0005408435,0.000016841652,0.00009454994,0.0000012928892],"about_ca_topic_score_codex":0.0033502835,"about_ca_topic_score_gemma":0.003322221,"teacher_disagreement_score":0.0033502835,"about_ca_system_score_codex":0.00026852483,"about_ca_system_score_gemma":0.00007097025,"threshold_uncertainty_score":0.006661594},"labels":[],"label_agreement":null},{"id":"W4289527479","doi":"10.3847/1538-4357/ac7a40","title":"Resolving the Inner Parsec of the Blazar J1924–2914 with the Event Horizon Telescope","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; McGill University; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Astrophysics Division; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; National Nuclear Security Administration; Toray Science Foundation; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Recruitment Program of Global Experts; European Research Council; Academy of Finland; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; Natural Sciences and Engineering Research Council of Canada; China Scholarship Council; John Templeton Foundation; European Southern Observatory; Ministry of Education, Culture, Sports, Science and Technology; Ministerio de Economía y Competitividad; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Harvard University; Radboud Universiteit; National Research Foundation; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Institutes of Natural Sciences; Government of Canada; Vetenskapsrådet; U.S. Department of Energy; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Simons Foundation; Compute Canada; National Astronomical Observatory of Japan; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Aeronautics and Space Administration; Department of Science and Technology, Ministry of Science and Technology, India; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Physics; Very-long-baseline interferometry; Blazar; Very Long Baseline Array; Astrophysics; Position angle; Supermassive black hole; Active galactic nucleus; Telescope; Astronomy; Galactic Center; Event horizon; Submillimeter Array; Galaxy; Event (particle physics); Gamma ray; Star formation","score_opus":0.005551660993071542,"score_gpt":0.19606010317676048,"score_spread":0.19050844218368895,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4289527479","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98903453,0.00019104576,0.0013227934,0.0001264526,0.000015505057,0.000016232787,0.00263943,0.00022193421,0.0064320453],"genre_scores_gemma":[0.98615336,0.00012402702,0.0051948014,0.000066688546,0.00004945975,0.00001685382,0.0071424274,0.00011275054,0.0011396537],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986625,0.00000795355,0.000004189971,0.0000355375,0.000047641362,0.000038368187],"domain_scores_gemma":[0.9997595,0.00002734376,0.00006875526,0.000027700216,0.000034935834,0.00008177513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023391447,0.00027786032,0.00025541594,0.0011757542,0.00035361538,0.0006179435,0.00030754978,0.00020590215,0.0037959053],"category_scores_gemma":[0.00027312234,0.00023518984,0.00022616057,0.0006490756,0.00013277099,0.00028697745,0.0005816532,0.00032502375,0.0006440802],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068476406,0.00040466464,0.45320255,0.000109958455,0.00041220206,0.0010948043,0.0007130977,0.0033154693,0.44649914,0.002838585,0.013451787,0.07727304],"study_design_scores_gemma":[0.000022440432,0.000025328141,0.99334174,0.0000055709374,0.000021439231,0.00008283484,0.000061840474,0.001111085,0.0019355492,0.00022447614,0.0031590012,0.000008741809],"about_ca_topic_score_codex":0.005725801,"about_ca_topic_score_gemma":0.01627821,"teacher_disagreement_score":0.005725801,"about_ca_system_score_codex":0.00033668402,"about_ca_system_score_gemma":0.00028444853,"threshold_uncertainty_score":0.012698531},"labels":[],"label_agreement":null},{"id":"W4289755583","doi":"10.3847/1538-4357/ac77fd","title":"The ALMaQUEST Survey. VIII. What Causes the Discrepancy in the Velocity between the CO and Hα Rotation Curves in Galaxies?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; Ministry of Science and Technology, Taiwan; Academia Sinica","keywords":"Galaxy rotation curve; Physics; Galaxy; Astrophysics; Rotation (mathematics); Velocity dispersion; Geometry; Galaxy formation and evolution; Mathematics","score_opus":0.014487535333599713,"score_gpt":0.24932940441254045,"score_spread":0.23484186907894072,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4289755583","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941193,0.00094700424,0.00015792596,0.00034348728,0.000024592426,0.0000069172693,0.0015439154,0.00003335622,0.002823421],"genre_scores_gemma":[0.99749845,0.00014113648,0.00020860948,0.00009824812,0.000042718224,0.0000061310284,0.0014864034,0.000012046977,0.0005063366],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993554,0.00011783561,0.000025033656,0.00026226652,0.0001418893,0.000097596596],"domain_scores_gemma":[0.99821126,0.00018355095,0.0008584503,0.00014236639,0.0003727978,0.00023155888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00074408675,0.00014864843,0.00022964022,0.0013897927,0.00035943463,0.000797981,0.0005334648,0.0003364437,0.0016543296],"category_scores_gemma":[0.0019334152,0.00010778632,0.00020815265,0.0011666523,0.00030632544,0.00065733155,0.00040931668,0.00020979346,0.0004932264],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037656268,0.000006492532,0.9940352,0.0000093317685,0.000017294542,0.0000463351,0.00006883851,0.000047371566,0.00039218008,0.00009406632,0.0006278996,0.0046173874],"study_design_scores_gemma":[0.000003625689,0.000009381651,0.9980914,0.0000054174966,0.0000058056885,0.000052380317,0.00013241172,0.00033300594,0.00008929119,0.00004635738,0.0012288262,0.0000020417933],"about_ca_topic_score_codex":0.021333024,"about_ca_topic_score_gemma":0.03916593,"teacher_disagreement_score":0.021333024,"about_ca_system_score_codex":0.00069914025,"about_ca_system_score_gemma":0.00023541464,"threshold_uncertainty_score":0.042417705},"labels":[],"label_agreement":null},{"id":"W4290666152","doi":"10.3847/1538-4357/ac6acf","title":"Searches for Gravitational Waves from Known Pulsars at Two Harmonics in the Second and Third LIGO-Virgo Observing Runs","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Université de Montréal; Canadian Institute for Theoretical Astrophysics; Polytechnique Montréal; University of British Columbia; University of Toronto; Perimeter Institute","funders":"European Social Fund; Astrophysics Division; Astrophysics Science Division; Division of Human Resource Development; National Research, Development and Innovation Office; Institute for Cosmic Ray Research, University of Tokyo; Science and Engineering Research Board; Japan Society for the Promotion of Science; McGill Space Institute; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; Canadian Institute for Advanced Research; National Astronomical Observatory of Japan; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Fondation familiale Trottier; Ministry of Education, India; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Nuclear Safety and Security Commission; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Hungarian Scientific Research Fund; University of Toronto; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; McGill University; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; U.S. Department of Energy; Smithsonian Institution; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Great Southern Development Commission, Government of Western Australia; Agencia Estatal de Investigación; Govern de les Illes Balears; Korea Institute of Science and Technology Information; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Culture, Sports, Science and Technology; European Regional Development Fund; ICTP South American Institute for Fundamental Research; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; Russian Science Foundation; University of British Columbia; Scottish Funding Council; Engineering and Physical Sciences Research Council; European Commission; Leverhulme Trust; National Science Foundation; Fundacja na rzecz Nauki Polskiej; Compute Canada; Western Canada Research Grid; Centres de Recerca de Catalunya; Institut des Origines de Lyon; University of Pennsylvania; National Aeronautics and Space Administration; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Ministerio de Ciencia e Innovación","keywords":"Physics; Pulsar; LIGO; Gravitational wave; Millisecond pulsar; Astrophysics; Quadrupole; Amplitude; Crab Pulsar; Harmonic number; Binary pulsar; Vela; Astronomy; Quantum mechanics","score_opus":0.029493018199804637,"score_gpt":0.3223808238601672,"score_spread":0.29288780566036254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4290666152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984635,0.00004563057,0.0004486027,0.000019626137,0.0000021652704,0.0000064029355,0.00050539087,0.000025714608,0.00048306226],"genre_scores_gemma":[0.9974293,0.00002517671,0.0008538594,0.000022929034,0.0000052575933,0.000010000422,0.0015119871,0.000012077626,0.00012952885],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99908555,0.00014450356,0.00004442827,0.00016218596,0.00030550966,0.00025789035],"domain_scores_gemma":[0.99760664,0.0005377468,0.00081173313,0.0003334316,0.00017176509,0.00053872133],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009248195,0.00041243035,0.00066878233,0.0020364677,0.00063363946,0.0013001349,0.00035378634,0.00047926707,0.0007165181],"category_scores_gemma":[0.0020516103,0.00025157793,0.0008633984,0.0014083405,0.00043206624,0.00029401292,0.0016565416,0.00048450465,0.0002351811],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010570156,0.00009495591,0.9547224,0.000029313056,0.0003415635,0.00035688598,0.0004126054,0.0019805701,0.030386522,0.0002698019,0.0003284709,0.010019912],"study_design_scores_gemma":[0.000036008758,0.00017691134,0.9898762,0.000010058244,0.00010409111,0.0002816876,0.00019257537,0.0022571755,0.005916149,0.00024412533,0.000879407,0.000025686977],"about_ca_topic_score_codex":0.0054780925,"about_ca_topic_score_gemma":0.010969562,"teacher_disagreement_score":0.0054780925,"about_ca_system_score_codex":0.00060912356,"about_ca_system_score_gemma":0.00043526816,"threshold_uncertainty_score":0.010892391},"labels":[],"label_agreement":null},{"id":"W4292056894","doi":"10.3847/1538-4357/ac7c1d","title":"The Photon Ring in M87*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":62,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Supermassive black hole; Astrophysics; Black hole (networking); Photon; Galaxy; Rest frame; Ring (chemistry); Astronomy; Redshift; Quantum mechanics","score_opus":0.011533071734654333,"score_gpt":0.22739738056124983,"score_spread":0.2158643088265955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292056894","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977658,0.000055238223,0.0011595656,0.00001800812,0.0000031840589,0.0000036585016,0.00013523993,0.000043716747,0.00081561593],"genre_scores_gemma":[0.99911886,0.000014739924,0.0006272939,0.000009036934,0.0000047015665,0.0000025419251,0.00013991214,0.000008606024,0.00007444282],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998574,0.000018771036,0.000004419042,0.000035152087,0.000044989374,0.00003924608],"domain_scores_gemma":[0.99957055,0.000051651998,0.0001748088,0.00008319551,0.000046792746,0.00007292955],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027281084,0.00021156942,0.0002836369,0.0005034704,0.00022752206,0.00046147915,0.00028901233,0.00019506332,0.00052559335],"category_scores_gemma":[0.00045861487,0.00015710785,0.00024546776,0.00027990792,0.00029060824,0.0001928914,0.0005542561,0.00026417262,0.00022417663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005306974,0.00007104198,0.65356886,0.00008975634,0.00018786079,0.0014145568,0.0010354737,0.0045363787,0.31065246,0.0017183245,0.0013147701,0.02487986],"study_design_scores_gemma":[0.000013451663,0.00014444588,0.96841097,0.000014398315,0.000049816532,0.00050444726,0.00015974801,0.0077154157,0.020908859,0.0003589456,0.0017044054,0.000015010106],"about_ca_topic_score_codex":0.0008322892,"about_ca_topic_score_gemma":0.0010724666,"teacher_disagreement_score":0.0008322892,"about_ca_system_score_codex":0.00023285905,"about_ca_system_score_gemma":0.00009100402,"threshold_uncertainty_score":0.0017582774},"labels":[],"label_agreement":null},{"id":"W4292057088","doi":"10.3847/1538-4357/ac7d4a","title":"Turbulence and Accretion: A High-resolution Study of the B5 Filaments","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Toronto; Herzberg Institute of Astrophysics; Queen's University","funders":"","keywords":"Protein filament; Physics; Turbulence; Astrophysics; Kinematics; Context (archaeology); Accretion (finance); Star formation; Velocity dispersion; Mechanics; Classical mechanics; Geology; Materials science; Galaxy","score_opus":0.009930699805199528,"score_gpt":0.2283668081318893,"score_spread":0.21843610832668978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292057088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99619603,0.00026167938,0.0017300834,0.000027107455,0.0000038319095,0.000007076037,0.00030479548,0.000084723935,0.0013846561],"genre_scores_gemma":[0.99831414,0.000057557554,0.0011932568,0.000011657005,0.0000055298497,0.0000025209945,0.00027947107,0.000009684479,0.00012630648],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996245,0.0000030026415,0.0000015216457,0.000010590486,0.000008471588,0.000013935676],"domain_scores_gemma":[0.9998809,0.000018390436,0.00003464936,0.000011290368,0.000019522897,0.000035187055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010661191,0.00015370875,0.00016964627,0.0008445973,0.0003489215,0.00038149368,0.00023927703,0.000187646,0.0010355006],"category_scores_gemma":[0.00019628387,0.00016765193,0.00022385368,0.00051558873,0.00017605034,0.0002384412,0.00029522777,0.0002270897,0.00018945152],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055950705,0.00023846248,0.22672158,0.00012308499,0.00020306664,0.0015813502,0.000516435,0.009670896,0.7321647,0.001421298,0.00071346,0.026086198],"study_design_scores_gemma":[0.0000189853,0.000101301535,0.96729016,0.000018661181,0.000032157583,0.0004298884,0.00023193947,0.01895236,0.01144732,0.00030559683,0.0011526513,0.000019077976],"about_ca_topic_score_codex":0.007389795,"about_ca_topic_score_gemma":0.005491201,"teacher_disagreement_score":0.007389795,"about_ca_system_score_codex":0.00021823873,"about_ca_system_score_gemma":0.00011819185,"threshold_uncertainty_score":0.014693558},"labels":[],"label_agreement":null},{"id":"W4292405826","doi":"10.3847/1538-4357/ac6877","title":"Magnetic Field Strength from Turbulence Theory. I. Using Differential Measure Approach","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":38,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Los Alamos National Laboratory; Nuclear Safety and Security Commission; University of Wisconsin-Madison; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Measure (data warehouse); Turbulence; Differential (mechanical device); Field (mathematics); Magnetic field; Statistical physics; Theoretical physics; Astrophysics; Mechanics; Quantum mechanics","score_opus":0.008296797954061153,"score_gpt":0.20622771482891925,"score_spread":0.1979309168748581,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292405826","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.059397087,0.008646713,0.8993179,0.0010591702,0.00053696084,0.00007757381,0.00041614578,0.00027656037,0.030271914],"genre_scores_gemma":[0.9266295,0.0041624974,0.06106636,0.00028393522,0.0006486945,0.00012767913,0.0003025405,0.00011522151,0.0066634235],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99983454,0.000060115337,0.00000922787,0.000028683511,0.000048904425,0.000018590817],"domain_scores_gemma":[0.9996598,0.00011774836,0.00007338056,0.000036890986,0.000076201104,0.000035992034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041324281,0.00058146147,0.00053418014,0.0015343553,0.00032957,0.0012893492,0.0007886765,0.00045341038,0.0010777321],"category_scores_gemma":[0.0012148214,0.00019100594,0.00045482765,0.00082767324,0.0010194761,0.001115867,0.00090049853,0.0006899744,0.0003169744],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003028825,0.00002887282,0.0022417724,0.00023049834,0.000047191763,0.00023134884,0.000083806895,0.070373856,0.0093507,0.88854027,0.0017556901,0.027085742],"study_design_scores_gemma":[0.000008197223,0.000029198274,0.0017560826,0.00003568625,0.000012113103,0.00014716292,0.000034937428,0.74082845,0.001449953,0.2514543,0.0042129727,0.00003097086],"about_ca_topic_score_codex":0.001360483,"about_ca_topic_score_gemma":0.0007084909,"teacher_disagreement_score":0.0015343553,"about_ca_system_score_codex":0.000953489,"about_ca_system_score_gemma":0.0002846919,"threshold_uncertainty_score":0.0069181323},"labels":[],"label_agreement":null},{"id":"W4292420463","doi":"10.3847/1538-4357/acb3c2","title":"Target Selection and Validation of DESI Quasars","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":190,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Division of Astronomical Sciences; Jet Propulsion Laboratory; National Taiwan University; Ministerio de Ciencia e Innovación; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Chinese Academy of Sciences; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; Gordon and Betty Moore Foundation; Consejo Nacional de Ciencia y Tecnología; National Science Foundation","keywords":"Quasar; Physics; Astrophysics; Redshift; Luminosity function; OVV quasar; QSOS; Galaxy; Astronomy; Dark matter; Luminosity; Stars","score_opus":0.009849332136353969,"score_gpt":0.2238219795007642,"score_spread":0.21397264736441024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292420463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95273405,0.000120255616,0.037003912,0.00006428354,0.000029132932,0.00029529873,0.0034794314,0.0022533892,0.0040202513],"genre_scores_gemma":[0.9512164,0.00004304264,0.031311445,0.000093975956,0.000025171714,0.00022124538,0.014821515,0.00028549484,0.0019817874],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9983601,0.00039277287,0.00008726946,0.00038314794,0.0005006257,0.000276137],"domain_scores_gemma":[0.9952146,0.001042461,0.00046581213,0.0009270643,0.0019361937,0.00041391843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003495326,0.00071251317,0.0005838038,0.0017059548,0.000541148,0.0007043325,0.0009137218,0.00047024447,0.0017552025],"category_scores_gemma":[0.0041503035,0.00026437998,0.0005153529,0.0008072158,0.00022460344,0.00037730252,0.001245864,0.00030668222,0.0015017428],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012682871,0.0007063071,0.7406139,0.00015709175,0.00027319565,0.00032212486,0.0005032107,0.027935501,0.06352746,0.0011001199,0.009092103,0.1545008],"study_design_scores_gemma":[0.0002976585,0.0010006313,0.5869859,0.00003944404,0.00020549467,0.00052270095,0.00042691623,0.24968365,0.14389649,0.0008859802,0.015979974,0.00007511573],"about_ca_topic_score_codex":0.0029353732,"about_ca_topic_score_gemma":0.0032508592,"teacher_disagreement_score":0.003495326,"about_ca_system_score_codex":0.00041856302,"about_ca_system_score_gemma":0.00032360305,"threshold_uncertainty_score":0.018485248},"labels":[],"label_agreement":null},{"id":"W4292421555","doi":"10.3847/1538-4357/acb3c0","title":"Overview of the DESI Milky Way Survey","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":136,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; University of Toronto","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Ministerio de Ciencia e Innovación; Ministry of Science and Technology, Taiwan; European Research Council; Nuclear Safety and Security Commission; National Tsing Hua University; Ministry of Education, India; U.S. Department of Energy; European Commission; National Science Foundation; Imperial College London; National Aeronautics and Space Administration","keywords":"Physics; Milky Way; Astronomy; Astrophysics; Stars","score_opus":0.04685100390346107,"score_gpt":0.26982884547059244,"score_spread":0.22297784156713135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292421555","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.19919795,0.012158637,0.01525439,0.003498828,0.000245227,0.000938459,0.64346343,0.0052737524,0.11996939],"genre_scores_gemma":[0.21579614,0.007435815,0.053025197,0.001632166,0.000490005,0.0015166922,0.6890346,0.0010783114,0.029991094],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99927527,0.000085496984,0.000064129374,0.00021162644,0.00025133204,0.000112190486],"domain_scores_gemma":[0.99850684,0.0001147826,0.00034027844,0.00024246167,0.00053971395,0.00025588254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011381307,0.00057298824,0.00038306878,0.00567922,0.00034078554,0.0008576779,0.0007479909,0.00026349069,0.007882596],"category_scores_gemma":[0.0014254391,0.00036013572,0.00031864017,0.0063174316,0.00014572618,0.0007584923,0.0014617222,0.0003467468,0.0049257935],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021612256,0.000079071724,0.4740087,0.0008455192,0.00017386732,0.000141152,0.0005828057,0.0015234026,0.0047476618,0.004007494,0.24324988,0.27042434],"study_design_scores_gemma":[0.000020528452,0.00003764837,0.4905909,0.00013742234,0.000035341374,0.00016740934,0.000214981,0.00069665804,0.0012591295,0.00070467574,0.5061106,0.00002467635],"about_ca_topic_score_codex":0.024190355,"about_ca_topic_score_gemma":0.022117306,"teacher_disagreement_score":0.024190355,"about_ca_system_score_codex":0.0012179612,"about_ca_system_score_gemma":0.0011624724,"threshold_uncertainty_score":0.0480991},"labels":[],"label_agreement":null},{"id":"W4292601840","doi":"10.3847/1538-4357/ac8056","title":"Limits on X-Ray Polarization at the Core of Centaurus A as Observed with the Imaging X-Ray Polarimetry Explorer","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Marshall Space Flight Center; Agenzia Spaziale Italiana","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Centaurus A; Polarimetry; Scattering; Population; Spectral line; Galaxy; Photon; Radio galaxy; Astronomy; Optics","score_opus":0.024806208632960024,"score_gpt":0.23243749737473973,"score_spread":0.20763128874177972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292601840","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980357,0.00013259072,0.00065314374,0.00001540768,0.0000027175508,0.0000018994862,0.00012566229,0.00003384481,0.0009989954],"genre_scores_gemma":[0.9995192,0.00003999256,0.00019618815,0.0000096535705,0.000006281985,0.000002514984,0.00016705431,0.0000054491925,0.00005346923],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996809,0.00006245297,0.000024058712,0.000073757255,0.00008865324,0.000070159054],"domain_scores_gemma":[0.99840516,0.00048302274,0.00045872654,0.00023313602,0.00019241693,0.0002275472],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007663851,0.00040850823,0.00028549996,0.0015495531,0.00039774983,0.0012835236,0.0003150222,0.0004249221,0.00074376026],"category_scores_gemma":[0.0018381235,0.00030679716,0.00032857174,0.00037057872,0.0004808646,0.0006399137,0.0010591686,0.0003098096,0.00031130094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096060376,0.000065526256,0.79108167,0.000051263938,0.00018454586,0.00029723966,0.00039772957,0.0019024797,0.19415082,0.0010065614,0.0002950624,0.009606445],"study_design_scores_gemma":[0.00001634245,0.00013934309,0.97777474,0.00002077102,0.00005288368,0.00030998667,0.00012435994,0.003272957,0.016990714,0.00063205446,0.00064255024,0.000023241906],"about_ca_topic_score_codex":0.000883433,"about_ca_topic_score_gemma":0.00066363637,"teacher_disagreement_score":0.0015495531,"about_ca_system_score_codex":0.00022895221,"about_ca_system_score_gemma":0.000078812474,"threshold_uncertainty_score":0.0040530562},"labels":[],"label_agreement":null},{"id":"W4292602186","doi":"10.3847/1538-4357/ac7b2e","title":"Metal Lines Associated with the Lyα Forest from eBOSS Data","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; China Scholarship Council; Ministry of Education, Science and Technology; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Carnegie Institution for Science; Leibniz-Gemeinschaft; University of Notre Dame; Ohio State University; National Research Foundation; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; National Research Foundation of Korea; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Quasar; Redshift; Astrophysics; Spectral line; Ionization; Galaxy; Baryon; Lyman-alpha forest; Metal; Absorption (acoustics); Flux (metallurgy); Intergalactic medium; Atomic physics; Astronomy; Ion; Chemistry; Optics","score_opus":0.015219226075332704,"score_gpt":0.21842471219603057,"score_spread":0.20320548612069786,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292602186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971194,0.00011532112,0.00030957125,0.000013082726,0.0000028494462,0.0000035348212,0.0012480005,0.000074284566,0.0011139195],"genre_scores_gemma":[0.99617565,0.0000649851,0.0005035471,0.000010145612,0.000008001834,0.000003026242,0.0030277276,0.000018294524,0.00018867059],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999169,0.0000044695826,0.0000056965846,0.000020870553,0.000026437328,0.000025509124],"domain_scores_gemma":[0.99976355,0.000027738526,0.00009120667,0.00002922932,0.000046856803,0.000041416417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016959225,0.00028358688,0.00015879648,0.0013124552,0.00017251645,0.0004256386,0.00017552836,0.00015796904,0.0011298556],"category_scores_gemma":[0.00032160053,0.00010619763,0.00021904947,0.000932711,0.0001630598,0.00027974998,0.00033259415,0.00014038142,0.00032918752],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003281112,0.00004708437,0.9040257,0.00011984812,0.00013204459,0.0005564976,0.00026819258,0.0026161377,0.06843817,0.00032911028,0.0011361225,0.02200303],"study_design_scores_gemma":[0.000007150191,0.000026747592,0.9904917,0.000009204865,0.00004727284,0.00011090334,0.00009146032,0.0033518057,0.0040737805,0.00009150857,0.001692167,0.0000062489503],"about_ca_topic_score_codex":0.004574238,"about_ca_topic_score_gemma":0.007083474,"teacher_disagreement_score":0.004574238,"about_ca_system_score_codex":0.00013304575,"about_ca_system_score_gemma":0.0000798909,"threshold_uncertainty_score":0.009095252},"labels":[],"label_agreement":null},{"id":"W4292602907","doi":"10.3847/1538-4357/ac8103","title":"Linking Small-scale Solar Wind Properties with Large-scale Coronal Source Regions through Joint Parker Solar Probe–Metis/Solar Orbiter Observations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Heliophysics Division; Science and Technology Facilities Council; Goddard Space Flight Center; Office of Experimental Program to Stimulate Competitive Research; Swedish National Space Agency; Uniwersytet Wrocławski; Office of Naval Research; Bundesministerium für Wirtschaft und Energie; National Science Foundation; Agenzia Spaziale Italiana; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; Istituto Nazionale di Astrofisica","keywords":"Physics; Solar wind; Coronal hole; Nanoflares; Orbiter; Corona (planetary geology); Heliosphere; Solar minimum; Astronomy; Astrophysics; Coronal mass ejection; Solar observatory; Solar cycle 23; Coronal loop; Solar cycle; Plasma; Magnetic field; Astrobiology; Venus","score_opus":0.025522247792067392,"score_gpt":0.20814686530135545,"score_spread":0.18262461750928807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292602907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808407,0.00006617043,0.00032485978,0.000013634612,0.0000036510826,0.000008215414,0.00053392514,0.000026808753,0.00093866384],"genre_scores_gemma":[0.9990388,0.000020585245,0.00029905533,0.000004832811,0.000005345263,0.000003664784,0.0005287342,0.0000054826523,0.00009344347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989593,0.000018104898,0.000006938858,0.00004035554,0.000021454505,0.000017183866],"domain_scores_gemma":[0.9996294,0.000088817666,0.000119962366,0.000040483457,0.00004344832,0.00007780088],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018578734,0.00017949544,0.00018030389,0.0008820402,0.00016887016,0.00048157835,0.00015939465,0.0002284215,0.0010010975],"category_scores_gemma":[0.00058786117,0.00011824664,0.00012995893,0.00065714173,0.00011009241,0.00028680597,0.0004479664,0.00016028213,0.00018868408],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023617788,0.000062652616,0.9414051,0.000044902303,0.00008051111,0.0002866364,0.00022248579,0.00097143336,0.04447246,0.00007913624,0.00042409365,0.011714265],"study_design_scores_gemma":[0.0000040515865,0.000021015798,0.9980211,0.0000018427396,0.0000062718336,0.000051477196,0.000039843755,0.0008251438,0.0008132321,0.000016756965,0.00019697426,0.0000022837628],"about_ca_topic_score_codex":0.0014890288,"about_ca_topic_score_gemma":0.004297757,"teacher_disagreement_score":0.0014890288,"about_ca_system_score_codex":0.00012059857,"about_ca_system_score_gemma":0.000063119616,"threshold_uncertainty_score":0.0033490062},"labels":[],"label_agreement":null},{"id":"W4292954620","doi":"10.3847/1538-4357/ac82b2","title":"On the Effects of Planetary Oblateness on Exoplanet Studies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Planet; Exoplanet; Oblate spheroid; RADIUS; Transit (satellite); Astrophysics; Equator; Earth radius; Astronomy; Classical mechanics; Latitude; Magnetosphere","score_opus":0.012662509933976836,"score_gpt":0.22476953377960454,"score_spread":0.2121070238456277,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4292954620","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9797887,0.00073546753,0.014203844,0.00057582074,0.000037841204,0.000023131468,0.00031837617,0.00017908729,0.0041376995],"genre_scores_gemma":[0.99795073,0.00011275804,0.0013814165,0.00008546414,0.00001642701,0.0000049185855,0.00014153024,0.00008239191,0.00022431221],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.98538786,0.009947285,0.0008571944,0.0014245445,0.001976386,0.0004067398],"domain_scores_gemma":[0.7410849,0.21034631,0.022986885,0.017503684,0.0066987737,0.0013794268],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.023118127,0.000558939,0.0005063525,0.0013695315,0.0007105122,0.0018130384,0.00048158775,0.000468479,0.0010138786],"category_scores_gemma":[0.13866238,0.00031859128,0.00070651196,0.0017393891,0.0016730631,0.0014351542,0.0018226252,0.0006876689,0.00035849697],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003076054,0.000021122494,0.96488035,0.000063146,0.00024207516,0.00036468447,0.0011496326,0.013455483,0.002774929,0.0007907958,0.00042011708,0.015530094],"study_design_scores_gemma":[0.000010290268,0.00017249375,0.9555901,0.00009840712,0.00015858939,0.00069788116,0.0006604382,0.029615885,0.007869761,0.0015414499,0.0035449055,0.000039622588],"about_ca_topic_score_codex":0.00707411,"about_ca_topic_score_gemma":0.0077139884,"teacher_disagreement_score":0.023118127,"about_ca_system_score_codex":0.0009556595,"about_ca_system_score_gemma":0.00055558,"threshold_uncertainty_score":0.12226176},"labels":[],"label_agreement":null},{"id":"W4293036718","doi":"10.3847/1538-4357/ac83c5","title":"The Mass Scale of High-redshift Galaxies: Virial Mass Estimates Calibrated with Stellar Dynamical Models from LEGA-C","year":2022,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Algorithm; Computer science","score_opus":0.0062687223359700565,"score_gpt":0.19034507575588935,"score_spread":0.1840763534199193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293036718","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9712539,0.00022209944,0.004570233,0.0002463559,0.0000143180705,0.000023547416,0.015763396,0.0008230257,0.0070831245],"genre_scores_gemma":[0.98362756,0.000030446314,0.0017521305,0.000044206365,0.000011247328,0.000015869202,0.014113273,0.00011265949,0.00029254524],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995521,0.00013077632,0.000019525747,0.0001398195,0.00007681779,0.000080956364],"domain_scores_gemma":[0.99636024,0.0009346214,0.0007584402,0.0010617396,0.0004264282,0.00045864086],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001656082,0.00042623022,0.00031540863,0.001735888,0.00036351557,0.0013918908,0.0009836325,0.00052327366,0.0021888835],"category_scores_gemma":[0.0037950217,0.00029413882,0.00080389134,0.0011114432,0.0003404344,0.0005358801,0.00091577996,0.00039738714,0.001440805],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004021658,0.00008486017,0.90485126,0.00006181928,0.00039770565,0.000104145336,0.00033552962,0.060536046,0.0048263352,0.0034623265,0.008092674,0.016845115],"study_design_scores_gemma":[0.000065061926,0.00003134067,0.90571094,0.000025563291,0.00007132991,0.00006173855,0.000093080904,0.084920496,0.0026004429,0.0014419369,0.004938917,0.00003912122],"about_ca_topic_score_codex":0.021849876,"about_ca_topic_score_gemma":0.013183099,"teacher_disagreement_score":0.021849876,"about_ca_system_score_codex":0.0015116906,"about_ca_system_score_gemma":0.0002976606,"threshold_uncertainty_score":0.04344541},"labels":[],"label_agreement":null},{"id":"W4293036898","doi":"10.3847/1538-4357/ac85e4","title":"The Ratio of Perpendicular and Parallel Diffusion Coefficients of Low-energy Particles in Turbulent Space Plasmas","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Magnetic confinement fusion research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics","score_opus":0.006330125063444259,"score_gpt":0.22239644435742537,"score_spread":0.2160663192939811,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293036898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7721304,0.0009271927,0.21238993,0.0005266975,0.00010107289,0.000036059584,0.00014911444,0.00048731396,0.013252172],"genre_scores_gemma":[0.9909634,0.0001851296,0.0061184806,0.000025910129,0.000018453442,0.0000100206835,0.00004819346,0.000060504197,0.002569928],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986124,0.000035953584,0.000006462607,0.000036019308,0.000038452064,0.00002189105],"domain_scores_gemma":[0.99946314,0.0002335153,0.00010808359,0.00004438043,0.000104614635,0.00004626477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035026725,0.00039190578,0.00019631027,0.00070086407,0.00022359517,0.0008337605,0.00033389765,0.00028316272,0.0014480851],"category_scores_gemma":[0.0019120816,0.00018350809,0.00022364399,0.00019397662,0.0007804597,0.0010342293,0.0005470896,0.0005304511,0.0002444483],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056514033,0.0001328138,0.018035851,0.00037863976,0.000094777,0.0008699645,0.00081056746,0.1390552,0.3754669,0.4301763,0.0024398724,0.031973943],"study_design_scores_gemma":[0.000038149105,0.000069035574,0.0082110325,0.000018571052,0.000017518532,0.0005176069,0.00010824773,0.880231,0.043678354,0.06445927,0.0025862432,0.000064961736],"about_ca_topic_score_codex":0.0010769397,"about_ca_topic_score_gemma":0.00031341647,"teacher_disagreement_score":0.0014480851,"about_ca_system_score_codex":0.00044288335,"about_ca_system_score_gemma":0.0002701655,"threshold_uncertainty_score":0.0048443675},"labels":[],"label_agreement":null},{"id":"W4293037023","doi":"10.3847/1538-4357/ac84dd","title":"Broadband X-Ray Spectroscopy and Estimation of Spin of the Galactic Black Hole Candidate GRS 1758–258","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Ministry of Science and Technology, Taiwan","keywords":"Physics; Astrophysics; Black hole (networking); Broadband; Spectroscopy; Intermediate-mass black hole; X-ray binary; Reflection (computer programming); Eddington luminosity; Spin-flip; Astronomy; Active galactic nucleus; Galaxy; Neutron star; Optics","score_opus":0.007734766802833918,"score_gpt":0.2353245305168077,"score_spread":0.2275897637139738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293037023","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995389,0.00005867468,0.0000627501,0.0000045157844,0.0000014470486,0.0000017365112,0.00007724698,0.0000055056057,0.00024924407],"genre_scores_gemma":[0.9995684,0.000016717497,0.00017262921,0.0000037328325,0.0000026671296,0.0000010716839,0.00012839594,0.0000015207357,0.00010502813],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995804,0.000003250587,0.0000032463056,0.000015367848,0.000009254561,0.000010835817],"domain_scores_gemma":[0.99987686,0.000010879586,0.000050304006,0.000011016737,0.000015737161,0.000035256042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001048043,0.00027861207,0.00019296756,0.0010821321,0.0002553614,0.00031893226,0.00017718066,0.00019083628,0.0008318091],"category_scores_gemma":[0.00023011169,0.000119311306,0.000117011135,0.00029585723,0.00015203578,0.00016499117,0.00024631855,0.00015440579,0.00027341442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048548644,0.00006892929,0.8296695,0.000040454797,0.00007081387,0.0014564074,0.0002528468,0.00048629346,0.15841484,0.00024896525,0.00020630733,0.008599166],"study_design_scores_gemma":[0.000010862586,0.00013073355,0.9931961,0.0000054381476,0.000026790205,0.0005849527,0.00016064392,0.00058268744,0.004620176,0.00006452337,0.0006107764,0.0000062382633],"about_ca_topic_score_codex":0.0012335265,"about_ca_topic_score_gemma":0.0019290108,"teacher_disagreement_score":0.0012335265,"about_ca_system_score_codex":0.00014430472,"about_ca_system_score_gemma":0.0000473927,"threshold_uncertainty_score":0.0027827024},"labels":[],"label_agreement":null},{"id":"W4293074991","doi":"10.3847/1538-4357/ac6dd9","title":"Multiwavelength Observations of the Blazar VER J0521+211 during an Elevated TeV Gamma-Ray State","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Institute for Cosmic Ray Research, University of Tokyo; Instituto de Astrofísica de Canarias; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Academy of Finland; Office of Science; University of Tokyo; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Max-Planck-Gesellschaft; Japan Society for the Promotion of Science; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministerio de Ciencia e Innovación; Hrvatska Zaklada za Znanost; Generalitat de Catalunya; National Research Centre; European Regional Development Fund; Bundesministerium für Bildung und Forschung; Ministry of Education, Culture, Sports, Science and Technology; National Energy Research Scientific Computing Center; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Smithsonian Institution; U.S. Department of Energy; Soochow University; Centres de Recerca de Catalunya; Deutsche Forschungsgemeinschaft; Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Blazar; Gamma ray; Astrophysics; Astronomy","score_opus":0.013192505795637877,"score_gpt":0.21373770571525716,"score_spread":0.20054519991961928,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293074991","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986468,0.00007555115,0.000088912486,0.000016972886,0.0000061906426,0.000004145315,0.0001907839,0.000017994134,0.00095272076],"genre_scores_gemma":[0.9989531,0.000042926422,0.00012960889,0.000020120513,0.000014871066,0.000004464648,0.0005548558,0.0000061824976,0.00027376777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998331,0.000015472273,0.000009460321,0.00003807862,0.00005540586,0.000048417278],"domain_scores_gemma":[0.99968266,0.000031910055,0.00012460128,0.000035199144,0.00004825664,0.000077331366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027139203,0.00023869528,0.0003738523,0.000818293,0.00075796654,0.0007308052,0.00025769247,0.00035351896,0.0006513256],"category_scores_gemma":[0.00039600683,0.0001877831,0.00031742587,0.000675791,0.00030798052,0.00021283072,0.0006579859,0.00036873287,0.00027344126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007603562,0.00021670242,0.8664896,0.000070700306,0.00019322758,0.0040408196,0.0008870719,0.00074865075,0.11074326,0.00021785994,0.0011199488,0.014511853],"study_design_scores_gemma":[0.0000040708455,0.000066670495,0.99761534,0.000005148294,0.000016899485,0.00036702643,0.00008995184,0.00020575892,0.00084832596,0.000017492526,0.0007575179,0.0000058417763],"about_ca_topic_score_codex":0.0038654506,"about_ca_topic_score_gemma":0.009413754,"teacher_disagreement_score":0.0038654506,"about_ca_system_score_codex":0.0004681879,"about_ca_system_score_gemma":0.00018091507,"threshold_uncertainty_score":0.0076858997},"labels":[],"label_agreement":null},{"id":"W4293138498","doi":"10.3847/1538-4357/aca5f8","title":"DESI Observations of the Andromeda Galaxy: Revealing the Immigration History of Our Nearest Neighbor","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Perimeter Institute; University of Waterloo","funders":"Division of Astronomical Sciences; Science and Technology Facilities Council; Canadian Space Agency; High Energy Physics; Smithsonian Astrophysical Observatory; Radcliffe Institute for Advanced Study, Harvard University; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Aspen Center for Physics; Harvard University; Simons Foundation; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; U.S. Department of Energy; Smithsonian Institution; Consejo Nacional de Ciencia y Tecnología; Ministerio de Ciencia e Innovación; John Simon Guggenheim Memorial Foundation","keywords":"Physics; Andromeda; Andromeda Galaxy; Astronomy; Astrophysics; Galaxy; k-nearest neighbors algorithm; Milky Way; Artificial intelligence","score_opus":0.03324961931771582,"score_gpt":0.23469173499393667,"score_spread":0.20144211567622083,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293138498","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975821,0.0000765095,0.00017409491,0.000024896415,0.0000013882225,0.0000025336744,0.00019962896,0.000019964162,0.0019187678],"genre_scores_gemma":[0.9989612,0.000037551854,0.00047995834,0.000010574818,0.000004201746,0.0000015553147,0.0002815221,0.0000044245567,0.00021909163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999312,0.000009150449,0.0000026039954,0.000019338626,0.000021700678,0.000015917216],"domain_scores_gemma":[0.9997769,0.00002556302,0.000060594026,0.00003770641,0.000027879645,0.000071385984],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016490355,0.00014734309,0.0001232497,0.00059589074,0.00040669032,0.00029298264,0.00015360779,0.00013112217,0.0009790158],"category_scores_gemma":[0.0002976629,0.0001010959,0.0001315713,0.0003619508,0.0001833047,0.00019914856,0.0005300193,0.0001751953,0.0003110061],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018119371,0.000046250316,0.9035016,0.000032313797,0.00006221203,0.00033864263,0.00075510493,0.0010605344,0.06956821,0.0008092561,0.0007007392,0.022943981],"study_design_scores_gemma":[0.000005777477,0.00004734561,0.99448496,0.000005304189,0.00000848219,0.00014820253,0.00014200277,0.0012146691,0.001858886,0.000113257025,0.0019645388,0.000006612309],"about_ca_topic_score_codex":0.004814235,"about_ca_topic_score_gemma":0.010467496,"teacher_disagreement_score":0.004814235,"about_ca_system_score_codex":0.0002546039,"about_ca_system_score_gemma":0.00009190411,"threshold_uncertainty_score":0.009572446},"labels":[],"label_agreement":null},{"id":"W4293182406","doi":"10.3847/1538-4357/ac83ab","title":"Polarized Synchrotron Foreground Assessment for CMB Experiments","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Cosmic microwave background; Galactic plane; Spectral index; Astrophysics; Synchrotron; Sky; Cosmic background radiation; Astronomy; Planck; Galaxy; Spectral line; Optics; Anisotropy","score_opus":0.016429683492554196,"score_gpt":0.28259976484719657,"score_spread":0.2661700813546424,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293182406","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9666146,0.00031036677,0.01641002,0.0002084004,0.000029681298,0.00008270115,0.006515283,0.00038694235,0.009441878],"genre_scores_gemma":[0.9862982,0.00008942008,0.0080617415,0.000099271674,0.00003854329,0.00006166377,0.0048145773,0.0000921745,0.00044448115],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99757,0.00082755677,0.00012251912,0.00037339487,0.0008304128,0.00027614273],"domain_scores_gemma":[0.98843014,0.003576357,0.0025259336,0.0025166832,0.0023519043,0.0005989684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0040659783,0.0004872105,0.00049541483,0.0028960044,0.00060890324,0.0019956573,0.00061479997,0.00057199213,0.0026511159],"category_scores_gemma":[0.007614509,0.0002705826,0.00047889992,0.0032954046,0.00033490796,0.0006776003,0.0012419589,0.0004978388,0.0005703339],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005552107,0.000093979776,0.9493166,0.00008862241,0.00018146182,0.00016653539,0.00021762712,0.005260631,0.012765425,0.0014127336,0.0015392441,0.028401943],"study_design_scores_gemma":[0.000020402273,0.0000919396,0.97553504,0.000035991157,0.00008144154,0.00014857536,0.0002854632,0.011844004,0.0066329003,0.0010175501,0.004286859,0.000019731197],"about_ca_topic_score_codex":0.00315448,"about_ca_topic_score_gemma":0.0040431283,"teacher_disagreement_score":0.0040659783,"about_ca_system_score_codex":0.0006628288,"about_ca_system_score_gemma":0.0003510748,"threshold_uncertainty_score":0.02150321},"labels":[],"label_agreement":null},{"id":"W4293212333","doi":"10.3847/1538-4357/ac8052","title":"The SOFIA FEEDBACK Legacy Survey Dynamics and Mass Ejection in the Bipolar H ii Region RCW 36","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Ames Research Center; Universität zu Köln; Deutsches Zentrum für Luft- und Raumfahrt; Universität Stuttgart; National Aeronautics and Space Administration; Agence Nationale de la Recherche; Universities Space Research Association; Armstrong Flight Research Center; Deutsche Forschungsgemeinschaft","keywords":"Physics; Astrophysics; Molecular cloud; Plasma; Nebula; Stars; Astronomy","score_opus":0.012448600487544387,"score_gpt":0.23017335469914102,"score_spread":0.21772475421159662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293212333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973037,0.00007220223,0.000060409784,0.000020668225,0.0000035130702,0.000004866775,0.0018070213,0.000037397098,0.00069013936],"genre_scores_gemma":[0.9976332,0.000037096106,0.00014978187,0.0000139636895,0.0000054491697,0.0000039602023,0.0020020155,0.000008915156,0.00014557313],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998857,0.000004925793,0.0000067987276,0.000035450423,0.000022922064,0.000044276992],"domain_scores_gemma":[0.99965537,0.0000140445045,0.00013306845,0.000039776318,0.00004755361,0.00011013093],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019981085,0.0002790265,0.00025578,0.0009025756,0.00024241653,0.0004636167,0.00023911052,0.00018092697,0.0007767133],"category_scores_gemma":[0.00038545372,0.00009825575,0.00022370668,0.0005836591,0.00014766306,0.00018470986,0.0004469736,0.00014600827,0.0002848442],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031172234,0.00004519909,0.96227694,0.000034068675,0.000098571574,0.00032381847,0.00029890236,0.00084448693,0.020479266,0.00007570853,0.001602049,0.013609171],"study_design_scores_gemma":[0.000003762947,0.000013212947,0.9986512,0.0000040908076,0.000011524076,0.000048522055,0.000047053192,0.00029455515,0.0004304615,0.000008270896,0.00048456163,0.0000028487768],"about_ca_topic_score_codex":0.026464049,"about_ca_topic_score_gemma":0.03116452,"teacher_disagreement_score":0.026464049,"about_ca_system_score_codex":0.00052154507,"about_ca_system_score_gemma":0.00021012798,"threshold_uncertainty_score":0.052619994},"labels":[],"label_agreement":null},{"id":"W4293214423","doi":"10.3847/1538-4357/ac82ee","title":"Cosmological Simulations of the Intergalactic Medium Evolution. III. SPH Simulations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; University of Victoria; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Galaxy formation and evolution; Astrophysics; Galaxy; Structure formation; Accretion (finance); Context (archaeology); Smoothed-particle hydrodynamics; Statistical physics; Algorithm","score_opus":0.010332506441352548,"score_gpt":0.22809348340830093,"score_spread":0.21776097696694838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293214423","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.60500723,0.00035043235,0.35357603,0.0008949091,0.00031999685,0.00037065227,0.003111709,0.0049628634,0.03140617],"genre_scores_gemma":[0.78427255,0.00016726262,0.20820291,0.00018883227,0.000055136108,0.00025341916,0.0018776685,0.00044738044,0.0045348518],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982446,0.00005592349,0.000011596233,0.000024063062,0.000056060726,0.000027944965],"domain_scores_gemma":[0.999373,0.00021772216,0.00005348885,0.00013379657,0.00014474586,0.00007724602],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005493687,0.00043618216,0.0004897906,0.00035461228,0.00036576725,0.0006769887,0.001230809,0.0008742898,0.0029883601],"category_scores_gemma":[0.0021130382,0.00025546123,0.00050756737,0.00056147395,0.0004717494,0.0007012258,0.0007527239,0.0007891543,0.00041826564],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011080356,0.000088564935,0.007057253,0.00006611356,0.0000854429,0.00012460617,0.00009713931,0.9615093,0.0047242967,0.012672183,0.0015976245,0.011866725],"study_design_scores_gemma":[0.00004333806,0.000011246832,0.0006255443,0.000002962356,0.0000043213936,0.000012160969,0.000008608464,0.99549073,0.0012002087,0.0012266038,0.0013699782,0.000004366395],"about_ca_topic_score_codex":0.01186395,"about_ca_topic_score_gemma":0.0068346118,"teacher_disagreement_score":0.01186395,"about_ca_system_score_codex":0.00082457915,"about_ca_system_score_gemma":0.0008294264,"threshold_uncertainty_score":0.02358979},"labels":[],"label_agreement":null},{"id":"W4293239474","doi":"10.3847/1538-4357/ac7f9e","title":"GaMPEN: A Machine-learning Framework for Estimating Bayesian Posteriors of Galaxy Morphological Parameters","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Vision and Imaging","field":"Computer Science","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Mila - Quebec Artificial Intelligence Institute","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Algorithm; Computer science","score_opus":0.01737350994222695,"score_gpt":0.28278771294515487,"score_spread":0.2654142030029279,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293239474","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0032516608,0.00018981635,0.9946743,0.00012709924,0.000013253875,0.000025323016,0.00015436934,0.0010996277,0.00046444795],"genre_scores_gemma":[0.20127587,0.00037930193,0.7934423,0.00036000845,0.00013178594,0.00035173158,0.001328015,0.0004675968,0.002263376],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9987747,0.0005877145,0.000044629553,0.0002616718,0.0002497245,0.000081627906],"domain_scores_gemma":[0.99611676,0.0026246116,0.0002983183,0.0003390734,0.00045906517,0.00016216747],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0055724555,0.0014856226,0.0015775197,0.002370873,0.0008785893,0.0019636343,0.0043429676,0.0018127527,0.0034659258],"category_scores_gemma":[0.013251517,0.0012513525,0.0013431399,0.001301043,0.0017364605,0.0022523487,0.002722431,0.0027284096,0.0008614037],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007552284,0.000029932382,0.0014293512,0.000055514243,0.00008439359,0.00007458327,0.000043861553,0.91140795,0.00057221885,0.03016375,0.0017757707,0.054287184],"study_design_scores_gemma":[0.0000044722633,0.0000039215984,0.00006894165,0.0000070447877,0.0000025230531,0.0000065201307,0.0000021478709,0.98668426,0.0001508994,0.012696822,0.00036868636,0.0000037496454],"about_ca_topic_score_codex":0.013840129,"about_ca_topic_score_gemma":0.015433208,"teacher_disagreement_score":0.013840129,"about_ca_system_score_codex":0.0019832256,"about_ca_system_score_gemma":0.0017781723,"threshold_uncertainty_score":0.029470325},"labels":[],"label_agreement":null},{"id":"W4293572274","doi":"10.3847/1538-4357/ac82f0","title":"Characterizing the 3D Kinematics of Young Stars in the Radcliffe Wave","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Kinematics; Stars; Astrophysics; Astronomy; Classical mechanics","score_opus":0.016411252187051556,"score_gpt":0.2241372119925923,"score_spread":0.20772595980554073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4293572274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978638,0.00003196507,0.0012747908,0.0000099329245,0.0000023410637,0.0000057690067,0.00014046469,0.000015937172,0.00065497565],"genre_scores_gemma":[0.99814963,0.000028193863,0.0012808496,0.000004530496,0.00000251154,0.0000039417114,0.00036212153,0.000010192061,0.00015805803],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999938,0.00000761059,0.0000039019806,0.000017788789,0.000016626862,0.000016103386],"domain_scores_gemma":[0.9996729,0.000047351972,0.000103902334,0.00004147962,0.000057544006,0.0000768358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018973676,0.0002423763,0.00019542372,0.0011663896,0.00017801617,0.0005557773,0.00024247292,0.00017511529,0.0006379833],"category_scores_gemma":[0.0006622179,0.00019977122,0.00033243818,0.000546062,0.00017810836,0.00023633809,0.0003956998,0.00015613488,0.00029921555],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001486946,0.000038492435,0.9532824,0.000017957547,0.00005876172,0.0002338808,0.00020010152,0.016911672,0.018067451,0.00089990103,0.0002529472,0.009887637],"study_design_scores_gemma":[0.0000133291305,0.00005150964,0.92119634,0.0000066995085,0.000016287828,0.00010384139,0.000118301075,0.07490253,0.002313494,0.00039251905,0.00087062735,0.000014609116],"about_ca_topic_score_codex":0.0059417845,"about_ca_topic_score_gemma":0.006970856,"teacher_disagreement_score":0.0059417845,"about_ca_system_score_codex":0.00037367753,"about_ca_system_score_gemma":0.00016823068,"threshold_uncertainty_score":0.011814415},"labels":[],"label_agreement":null},{"id":"W4294253306","doi":"10.3847/1538-4357/ac85bc","title":"The R-Process Alliance: Abundance Universality among Some Elements at and between the First and Second R-Process Peaks*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF","funders":"National Science Foundation; European Research Council; Horizon 2020 Framework Programme; U.S. Department of Energy; Los Alamos National Laboratory; Science and Technology Facilities Council","keywords":"r-process; Nucleosynthesis; Physics; Stars; Astrophysics; s-process; Abundance (ecology); Universality (dynamical systems)","score_opus":0.008874629237986077,"score_gpt":0.23059564275045097,"score_spread":0.2217210135124649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294253306","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948258,0.0001535639,0.0013509186,0.000036588164,0.000001962893,0.0000035680541,0.000097891105,0.000052207044,0.0034773345],"genre_scores_gemma":[0.9995053,0.000010101105,0.0003009248,0.000008658319,0.0000023495168,0.0000012592956,0.00006848755,0.000009674918,0.00009326839],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996049,0.000052461397,0.000021014326,0.00016697592,0.000097819735,0.000056872334],"domain_scores_gemma":[0.99819905,0.00037843027,0.00056879106,0.00043460005,0.00024296944,0.00017619667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096037716,0.00014335784,0.00029440224,0.0012314023,0.00036036837,0.0010823961,0.0005034589,0.00031602327,0.0010256848],"category_scores_gemma":[0.0024941973,0.00015028843,0.00031120007,0.0005142233,0.00063348666,0.0009307195,0.0014457757,0.00044063924,0.00030079237],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003901017,0.000037405087,0.93413407,0.000039319595,0.00008948028,0.00015053406,0.00055107515,0.0009521443,0.041142523,0.0054115904,0.00021347756,0.016888294],"study_design_scores_gemma":[0.000014187884,0.00019405536,0.9744271,0.000011642243,0.000034454224,0.0004754862,0.00032193447,0.0038193895,0.012922942,0.0052031623,0.002556557,0.000019093834],"about_ca_topic_score_codex":0.0009247177,"about_ca_topic_score_gemma":0.00092471717,"teacher_disagreement_score":0.0012314023,"about_ca_system_score_codex":0.00027086728,"about_ca_system_score_gemma":0.00015200156,"threshold_uncertainty_score":0.005079031},"labels":[],"label_agreement":null},{"id":"W4294686848","doi":"10.3847/1538-4357/ac7a3c","title":"Using Bayesian Deep Learning to Infer Planet Mass from Gaps in Protoplanetary Disks","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Planet; Physics; Bayesian probability; Astrophysics; Bayesian network; Artificial intelligence; Deep learning; Algorithm; Machine learning; Computer science","score_opus":0.01285088733715877,"score_gpt":0.24483461333765225,"score_spread":0.23198372600049347,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294686848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8169829,0.00064774125,0.17639178,0.0008094249,0.00006412926,0.00002563335,0.00064692635,0.0016765452,0.002754987],"genre_scores_gemma":[0.9867582,0.00006812907,0.01190015,0.00009061254,0.000017611937,0.000013293592,0.0005862441,0.000032192453,0.00053355587],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991393,0.000021122043,0.00000330034,0.000026069883,0.000019440788,0.000016122174],"domain_scores_gemma":[0.99940455,0.0003288112,0.000075485055,0.000042218886,0.000083138635,0.00006571991],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005711771,0.0004925752,0.0003223692,0.00048780203,0.00024667813,0.00044828185,0.0007782258,0.00070065935,0.00077639363],"category_scores_gemma":[0.0023768796,0.00032568973,0.0002633681,0.0002741725,0.00040709766,0.0007839899,0.0007102445,0.0008259204,0.00021799168],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011754213,0.00009521929,0.0116246315,0.000030909465,0.00004024052,0.00004505745,0.000029292105,0.9540993,0.0019525568,0.001460284,0.0012437487,0.02926132],"study_design_scores_gemma":[0.0000032886367,0.0000050624258,0.00050290773,0.0000019766087,0.000001565366,0.0000021115106,0.0000021617361,0.9982514,0.0002682569,0.00090252585,0.00005713056,0.0000016719855],"about_ca_topic_score_codex":0.008821722,"about_ca_topic_score_gemma":0.0071751117,"teacher_disagreement_score":0.008821722,"about_ca_system_score_codex":0.00071540696,"about_ca_system_score_gemma":0.0005344995,"threshold_uncertainty_score":0.017540753},"labels":[],"label_agreement":null},{"id":"W4294796203","doi":"10.3847/1538-4357/ac80fc","title":"Measuring the β-decay Properties of Neutron-rich Exotic Pm, Sm, Eu, and Gd Isotopes to Constrain the Nucleosynthesis Yields in the Rare-earth Region","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia; TRIUMF","funders":"Oak Ridge National Laboratory; National Research, Development and Innovation Office; Agencia Estatal de Investigación; RIKEN; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Nuclear Physics; Natural Sciences and Engineering Research Council of Canada; Narodowe Centrum Nauki; Ministerio de Ciencia e Innovación; National Nuclear Security Administration; Generalitat Valenciana; Agencia Nacional de Investigación y Desarrollo; Ministerio de Ciencia, Innovación y Universidades; Western Canada Research Grid; National Science Foundation; Compute Canada; TRIUMF; U.S. Department of Energy","keywords":"Physics; Nucleosynthesis; Isotope; Neutron; r-process; Nuclear physics; Abundance (ecology); Neutron capture; Neutron number; Nuclear reaction; Neutron temperature; Neutron cross section","score_opus":0.049524017037403195,"score_gpt":0.241050075135191,"score_spread":0.1915260580977878,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294796203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97910863,0.00028377274,0.018423758,0.00001945739,0.000007668092,0.000014890509,0.00019866039,0.000077059085,0.0018661466],"genre_scores_gemma":[0.99306715,0.00010867221,0.0064005214,0.000012840307,0.0000022481893,0.000012413295,0.00012237632,0.000021089321,0.00025270972],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99979395,0.00004960679,0.000012824298,0.00006389532,0.00006223575,0.000017526998],"domain_scores_gemma":[0.9995529,0.00017302968,0.00009523865,0.000055062053,0.00009949401,0.000024292558],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010236918,0.00041126608,0.00027216654,0.00059346657,0.00018856268,0.00037633767,0.00029279554,0.00023455788,0.00057877455],"category_scores_gemma":[0.00091819314,0.00027357662,0.00022991582,0.00028912368,0.0002567243,0.00036837236,0.00039183686,0.00025775662,0.00013422214],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005864988,0.000032432057,0.07216304,0.000093908646,0.00008896682,0.000119082775,0.00011482908,0.006275716,0.9102965,0.0010506734,0.000073251795,0.009105065],"study_design_scores_gemma":[0.00003912748,0.00036952092,0.08274909,0.000018527868,0.00011216388,0.0003651765,0.00008103877,0.047806397,0.8653833,0.00060105143,0.0024393103,0.000035352983],"about_ca_topic_score_codex":0.00065346516,"about_ca_topic_score_gemma":0.0014826371,"teacher_disagreement_score":0.0010236918,"about_ca_system_score_codex":0.00032350927,"about_ca_system_score_gemma":0.00012512138,"threshold_uncertainty_score":0.00541389},"labels":[],"label_agreement":null},{"id":"W4294796709","doi":"10.3847/1538-4357/ac886e","title":"NuSTAR Observations of Intrinsically X-Ray Weak Quasar Candidates: An Obscuration-only Scenario","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; National Natural Science Foundation of China; Pennsylvania State University; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; California Institute of Technology; University of Pennsylvania; Smithsonian Institution","keywords":"Physics; Algorithm; Computer science","score_opus":0.019119849906942418,"score_gpt":0.23974939677312748,"score_spread":0.22062954686618508,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294796709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9944781,0.0001300037,0.001306143,0.00006281401,0.0000042495462,0.0000055870314,0.00029680284,0.0000679803,0.0036482767],"genre_scores_gemma":[0.998075,0.0000358986,0.0006493027,0.000038460574,0.0000083616005,0.0000040600166,0.0006572134,0.000011642505,0.00052006],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986005,0.00001756117,0.000011213197,0.00003557305,0.00003866828,0.000037010803],"domain_scores_gemma":[0.9987968,0.00017665884,0.00046085202,0.00018901753,0.00012393175,0.00025264072],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053250155,0.00023508068,0.00035507875,0.0008347156,0.0002785303,0.0009705288,0.00039425227,0.00030095445,0.002204579],"category_scores_gemma":[0.0009179303,0.00022358452,0.00025139906,0.0005513109,0.00031983535,0.00047217743,0.0010610997,0.0002936583,0.00068565435],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029845006,0.000027421462,0.9344097,0.00007882757,0.00008282737,0.0006094687,0.0002950667,0.0009801273,0.04936584,0.0009927755,0.00050243974,0.012356964],"study_design_scores_gemma":[0.000018217586,0.000097708355,0.9878813,0.000013071425,0.000048168396,0.0004053597,0.00016609089,0.0032449965,0.005885854,0.0005077454,0.0017195237,0.000012034269],"about_ca_topic_score_codex":0.0010938367,"about_ca_topic_score_gemma":0.002770822,"teacher_disagreement_score":0.002204579,"about_ca_system_score_codex":0.0002675101,"about_ca_system_score_gemma":0.00010978734,"threshold_uncertainty_score":0.007375002},"labels":[],"label_agreement":null},{"id":"W4294875709","doi":"10.3847/1538-4357/ac84d0","title":"TIC 5724661: A Long-period Binary with a Pulsating sdB Star and δ Scuti Variable","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"Natural Sciences and Engineering Research Council of Canada; Narodowe Centrum Nauki","keywords":"Physics; Subdwarf; Astrophysics; Binary star; Common envelope; Orbital period; Astronomy; Amplitude; Radial velocity; Binary number; Stars; Variable star; Orbital eccentricity; Orbit (dynamics); Binary system; White dwarf","score_opus":0.007761235497096254,"score_gpt":0.2030280589355033,"score_spread":0.19526682343840704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4294875709","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99599236,0.000051348597,0.00022167865,0.00008024712,0.000016985196,0.000007778896,0.00021094565,0.000021656297,0.003397078],"genre_scores_gemma":[0.99825674,0.000014973855,0.00029598273,0.000035421603,0.000009234974,0.0000033732501,0.00040551764,0.00000460291,0.00097398274],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993825,0.000005979812,0.000006602669,0.000014541848,0.000018309274,0.000016306067],"domain_scores_gemma":[0.9997719,0.000026240523,0.000057282658,0.000019269477,0.000016568405,0.00010870141],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014946554,0.00016432485,0.0002198433,0.0007341428,0.0009931887,0.00052671,0.00024724466,0.00032794208,0.0031077836],"category_scores_gemma":[0.0003991623,0.000119908036,0.00008002083,0.000746413,0.00028321374,0.00020982245,0.00039246227,0.0003481894,0.00067413424],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015778149,0.00079492433,0.8285693,0.00010200131,0.00010781574,0.018666126,0.00055997027,0.0028668167,0.11034872,0.0055604326,0.004797316,0.026048739],"study_design_scores_gemma":[0.00023781674,0.0010819108,0.9126413,0.00003779365,0.00006666316,0.0245671,0.00078980665,0.01686555,0.021925576,0.0025700734,0.019169692,0.00004666149],"about_ca_topic_score_codex":0.002491149,"about_ca_topic_score_gemma":0.0037004484,"teacher_disagreement_score":0.0031077836,"about_ca_system_score_codex":0.00038537194,"about_ca_system_score_gemma":0.00024553423,"threshold_uncertainty_score":0.0103966},"labels":[],"label_agreement":null},{"id":"W4295047794","doi":"10.3847/1538-4357/ac854c","title":"The Physical Properties of Low-redshift FeLoBAL Quasars. III. The Location and Geometry of the Outflows","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; Western University","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; York University; Universität Basel; Fermilab; National Science Foundation; Case Western Reserve University; Carnegie Mellon University; University of Pittsburgh; Los Alamos National Laboratory; College of Engineering, Michigan State University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Princeton University; Aspen Center for Physics; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Drexel University; Vanderbilt University; University of Oklahoma; National Aeronautics and Space Administration; U.S. Naval Observatory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Outflow; Quasar; Redshift; Accretion (finance); Emission spectrum; Ionization; Spectral line; RADIUS; Doubly ionized oxygen; Astronomy; Galaxy; Ion","score_opus":0.007201519163787629,"score_gpt":0.19879151305090298,"score_spread":0.19158999388711534,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4295047794","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993437,0.000111970265,0.00007863005,0.000009237389,6.02478e-7,0.0000022824554,0.00012569217,0.0000035640962,0.0003242174],"genre_scores_gemma":[0.9996909,0.000026172944,0.000046016456,0.0000044842523,0.0000023265347,0.0000015318382,0.00015810189,0.0000013194268,0.00006917091],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998374,0.000024003575,0.000016812903,0.00003579597,0.000028576373,0.00005738752],"domain_scores_gemma":[0.99887127,0.0002278413,0.00049624406,0.000069956775,0.00012875171,0.00020584985],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051059946,0.0002534945,0.00026357637,0.0025997458,0.0004623534,0.0007986744,0.00029123813,0.00027724056,0.0015758805],"category_scores_gemma":[0.0012355385,0.00011403721,0.00020275175,0.000799842,0.0005737224,0.00038121067,0.00046556443,0.0002147286,0.00034243966],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031521195,0.000016111599,0.994846,0.0000066790626,0.000009576718,0.00006168202,0.000071267124,0.000044536275,0.0029705737,0.000047172074,0.00002077525,0.0018740677],"study_design_scores_gemma":[0.0000010102053,0.000018620067,0.99945086,0.0000015120988,0.000003352026,0.000101683596,0.000070962626,0.0000709146,0.00018062677,0.000024662406,0.000074301985,0.0000013520026],"about_ca_topic_score_codex":0.0019833285,"about_ca_topic_score_gemma":0.001959617,"teacher_disagreement_score":0.0025997458,"about_ca_system_score_codex":0.00026905147,"about_ca_system_score_gemma":0.00007118525,"threshold_uncertainty_score":0.005271852},"labels":[],"label_agreement":null},{"id":"W4295135046","doi":"10.3847/1538-4357/ac84d2","title":"Diagnosing FU Ori-like Sources: The Parameter Space of Viscously Heated Disks in the Optical and Near-infrared","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Photosphere; T Tauri star; Accretion (finance); Spectral line; Infrared; Stars; Spectral energy distribution; Photometry (optics); Astronomy; Galaxy","score_opus":0.012146765068909472,"score_gpt":0.24025510289672738,"score_spread":0.22810833782781792,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4295135046","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947889,0.000052394887,0.004205947,0.00003077955,8.5371556e-7,0.000014806773,0.00016078418,0.00010188991,0.0006437433],"genre_scores_gemma":[0.9972838,0.00002482544,0.0023328105,0.00000723934,0.0000027363603,0.0000070276787,0.0002616323,0.000010592794,0.0000693658],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99974483,0.00007395702,0.000015512096,0.00006907675,0.000047647027,0.000048966638],"domain_scores_gemma":[0.9987105,0.00068378,0.000279144,0.00015903176,0.00005826542,0.000109300716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007579398,0.0006981355,0.00036104806,0.0013821331,0.0003182258,0.0015686405,0.000789008,0.0008457828,0.00053884625],"category_scores_gemma":[0.0033294966,0.0003787955,0.00051165425,0.00077635364,0.00032487474,0.00095420924,0.00080778106,0.00023849987,0.0001685825],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024183957,0.000097999735,0.8767902,0.00003455473,0.00010308122,0.00052500796,0.0003470124,0.096961305,0.009136572,0.0013965701,0.00023758641,0.014128265],"study_design_scores_gemma":[0.0000703385,0.00012241553,0.43880418,0.000031618176,0.000109267465,0.0005567066,0.0010351207,0.5450143,0.009134778,0.0040532625,0.0010189234,0.000049016886],"about_ca_topic_score_codex":0.0051263063,"about_ca_topic_score_gemma":0.004061293,"teacher_disagreement_score":0.0051263063,"about_ca_system_score_codex":0.0006275136,"about_ca_system_score_gemma":0.00028590937,"threshold_uncertainty_score":0.010192931},"labels":[],"label_agreement":null},{"id":"W4295242307","doi":"10.3847/1538-4357/ac87a6","title":"Do All Low-Mass Stars Undergo Extra Mixing Processes?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Stars; Stellar evolution; RADIUS; Mixing (physics); Nebula; Planetary nebula; Galaxy; Red supergiant; Supergiant; Astronomy","score_opus":0.015340577258663167,"score_gpt":0.23401489594706515,"score_spread":0.21867431868840198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4295242307","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9695043,0.0018419856,0.004575887,0.0023656087,0.00014513687,0.000026330024,0.00043357996,0.00019048847,0.020916637],"genre_scores_gemma":[0.9972589,0.00016628264,0.0004458807,0.00024693244,0.00008835349,0.000004217964,0.00013804733,0.000015360227,0.0016359065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99957126,0.00006745721,0.00003096482,0.00014981088,0.00007035451,0.00011014046],"domain_scores_gemma":[0.99743736,0.00045397933,0.0008607483,0.000504625,0.0002507779,0.0004925493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001034865,0.00026720346,0.0004638647,0.0005114314,0.00066245114,0.0018255267,0.00062531687,0.00088642124,0.009874633],"category_scores_gemma":[0.0042747566,0.00018580187,0.00030334367,0.00051805924,0.0010535658,0.0023096718,0.0009524835,0.00056940375,0.002207647],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013765848,0.0001788616,0.81463534,0.0002842063,0.00016495459,0.0008468309,0.0009903077,0.00084448647,0.01769155,0.03203809,0.002879442,0.12806931],"study_design_scores_gemma":[0.0001387129,0.0003340184,0.8190551,0.00011134982,0.00014080341,0.0035047703,0.0016246336,0.006350945,0.014277926,0.12878586,0.025618047,0.00005785491],"about_ca_topic_score_codex":0.00080435106,"about_ca_topic_score_gemma":0.0006247581,"teacher_disagreement_score":0.009874633,"about_ca_system_score_codex":0.00041332497,"about_ca_system_score_gemma":0.0001708143,"threshold_uncertainty_score":0.033033967},"labels":[],"label_agreement":null},{"id":"W4295242329","doi":"10.3847/1538-4357/ac887d","title":"A New Census of the 0.2 &lt; z &lt; 3.0 Universe. II. The Star-forming Sequence","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":134,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Star formation; Metallicity; Redshift; Stellar population; Spectral energy distribution; Flattening; Galaxy formation and evolution; Population; Astronomy","score_opus":0.01132068531331644,"score_gpt":0.20880294931482216,"score_spread":0.1974822640015057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4295242329","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8597798,0.0009172784,0.0070162225,0.00061595964,0.00005072932,0.00006150888,0.11755698,0.0002878708,0.013713654],"genre_scores_gemma":[0.8815064,0.0010051379,0.009531073,0.00034272484,0.00007728375,0.000101154284,0.09980995,0.00016196443,0.007464367],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998909,0.000015461545,0.000006251236,0.000040186624,0.000029156867,0.000018008926],"domain_scores_gemma":[0.9996686,0.000037886435,0.00008149677,0.000058902693,0.000060279584,0.000092801114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002355121,0.00021282728,0.00016687078,0.0012100852,0.00022545696,0.0006188567,0.00018768232,0.00018750435,0.0053376937],"category_scores_gemma":[0.00086143566,0.00014790644,0.00020261163,0.0018131592,0.00014316099,0.0007138202,0.0005750336,0.00045217315,0.0015273315],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036233303,0.00016029926,0.71419364,0.00020316997,0.00015107916,0.0004736858,0.0019867704,0.0033369672,0.014420554,0.03122142,0.06279703,0.17069298],"study_design_scores_gemma":[0.000009457154,0.000036364407,0.92344576,0.000018211036,0.00001330687,0.0003116501,0.00021601377,0.0023668911,0.0010066907,0.0018013642,0.07075914,0.000015138312],"about_ca_topic_score_codex":0.016687896,"about_ca_topic_score_gemma":0.02197864,"teacher_disagreement_score":0.016687896,"about_ca_system_score_codex":0.00027820544,"about_ca_system_score_gemma":0.00019960194,"threshold_uncertainty_score":0.033181548},"labels":[],"label_agreement":null},{"id":"W4295366670","doi":"10.3847/1538-4357/ac89ec","title":"Asteroid Measurements at Millimeter Wavelengths with the South Pole Telescope","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"National Astronomical Observatory of Japan; Planetary Science Division; National Institutes of Natural Sciences; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Alfred P. Sloan Foundation; National Radio Astronomy Observatory; University of Chicago; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Asteroid; Physics; Telescope; Cosmic microwave background; Millimeter; Astrophysics; Astronomy; Light curve; Brightness; Sky; Ecliptic; Flux (metallurgy); Wavelength; Optics; Anisotropy","score_opus":0.015509070447342323,"score_gpt":0.19974351930627443,"score_spread":0.18423444885893211,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4295366670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9816305,0.0003698984,0.0075174933,0.0001321379,0.00003185064,0.000017728631,0.003120418,0.00048542718,0.0066945846],"genre_scores_gemma":[0.98928356,0.00011038348,0.0066330656,0.00004063396,0.00003314639,0.000015200102,0.0030600529,0.00003945928,0.00078445487],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997286,0.000020490834,0.0000072164235,0.00009109456,0.00012489635,0.000027655438],"domain_scores_gemma":[0.99955994,0.000047254507,0.00014450325,0.00007469398,0.000115208044,0.00005838626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002465399,0.00026862958,0.00030990594,0.0009597048,0.0003178756,0.00045846344,0.00033169385,0.00029256477,0.0017010503],"category_scores_gemma":[0.0005844544,0.00024240703,0.00025045167,0.00075165974,0.00014815232,0.00041159592,0.00045620525,0.00050212897,0.0008218529],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034040105,0.000054225056,0.66444725,0.00010360346,0.0001894963,0.00038667623,0.0007229814,0.0011905545,0.279205,0.0004500157,0.004786445,0.04812327],"study_design_scores_gemma":[0.0000129098435,0.000059802034,0.9830313,0.0000075504668,0.000026066715,0.0002953826,0.00006790426,0.0015694754,0.010595263,0.00010758106,0.004216659,0.000010253612],"about_ca_topic_score_codex":0.0019528302,"about_ca_topic_score_gemma":0.004440318,"teacher_disagreement_score":0.0019528302,"about_ca_system_score_codex":0.000317888,"about_ca_system_score_gemma":0.00010869607,"threshold_uncertainty_score":0.0056905746},"labels":[],"label_agreement":null},{"id":"W4295367350","doi":"10.3847/1538-4357/ac8b02","title":"A Rosetta Stone for Eccentric Gravitational Waveform Models","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":44,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"University of British Columbia Graduate School; Natural Sciences and Engineering Research Council of Canada; University of Cambridge; National Science Foundation","keywords":"Physics; Gravitation; Waveform; Astronomy; Gravitational wave; Astrophysics","score_opus":0.01944277098779095,"score_gpt":0.3151082591372079,"score_spread":0.29566548814941696,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4295367350","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.013917121,0.00022511177,0.9769254,0.00060560147,0.00008321276,0.000067202345,0.00014393764,0.0005291237,0.0075032217],"genre_scores_gemma":[0.21016987,0.00043669486,0.78331053,0.00022202502,0.00014421208,0.00045405835,0.0005282232,0.0007747189,0.0039596516],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9990652,0.00042080964,0.000070716465,0.000110063505,0.0002691645,0.00006401532],"domain_scores_gemma":[0.99542075,0.0020826163,0.00033470948,0.0013931878,0.0005964913,0.00017215309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003939731,0.0007039785,0.0009620608,0.0012190907,0.0009228561,0.0020345584,0.003710666,0.0014680709,0.0048621725],"category_scores_gemma":[0.01229551,0.0009162617,0.0019833115,0.0006771836,0.0014418104,0.0031697447,0.0034822277,0.0026889825,0.0011489962],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034819266,0.00005410774,0.0010809212,0.00005651601,0.00005625735,0.00007935632,0.0001361852,0.2271186,0.00091122225,0.75387865,0.0014045319,0.015188864],"study_design_scores_gemma":[0.000012722073,0.000018444358,0.000107283595,0.00003133457,0.000011226837,0.000042086693,0.000021753749,0.7908049,0.00029785122,0.20298976,0.005646466,0.000016188815],"about_ca_topic_score_codex":0.0034920287,"about_ca_topic_score_gemma":0.003866692,"teacher_disagreement_score":0.0048621725,"about_ca_system_score_codex":0.0009989433,"about_ca_system_score_gemma":0.0011389956,"threshold_uncertainty_score":0.020835519},"labels":[],"label_agreement":null},{"id":"W4295941398","doi":"10.3847/1538-4357/ac8a48","title":"The JCMT Transient Survey: Single-epoch Transients and Variability of Faint Sources","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Flare; Astronomy; Variable star; Submillimeter Array; Star formation; Galaxy; Stars","score_opus":0.013664757730841411,"score_gpt":0.22285248555170678,"score_spread":0.20918772782086537,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4295941398","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99857795,0.000053813674,0.00013569446,0.000012757475,0.0000019879496,0.000005701519,0.0008273524,0.000019541276,0.00036525863],"genre_scores_gemma":[0.9973436,0.000037320635,0.00025905608,0.000008983918,0.000014210576,0.000005318807,0.0021260635,0.000008891097,0.0001965603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982375,0.000010121528,0.00001596957,0.000048457707,0.000049594742,0.00005214384],"domain_scores_gemma":[0.9985461,0.0001408651,0.0007050688,0.0001533074,0.00013427295,0.0003204453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025225212,0.00017506388,0.00027297786,0.0023138633,0.00039879393,0.0006045953,0.0003234895,0.00028282544,0.0011309781],"category_scores_gemma":[0.0010523229,0.000114855146,0.00025893078,0.0015169992,0.00020311357,0.0004472619,0.00063256995,0.00020552792,0.00026739918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000086643304,0.000040280967,0.9855612,0.000016578451,0.00003451998,0.0001542988,0.00012948162,0.00020661486,0.008317829,0.00004991656,0.00033762533,0.0050649256],"study_design_scores_gemma":[0.0000015350488,0.0000118770995,0.99914324,0.0000016025173,0.000006166826,0.00008109221,0.000024698447,0.00024716769,0.00031614013,0.00000549262,0.00015972016,0.0000012259255],"about_ca_topic_score_codex":0.007628274,"about_ca_topic_score_gemma":0.01348833,"teacher_disagreement_score":0.007628274,"about_ca_system_score_codex":0.0002852026,"about_ca_system_score_gemma":0.00020136402,"threshold_uncertainty_score":0.015167713},"labels":[],"label_agreement":null},{"id":"W4296066750","doi":"10.3847/1538-4357/ac8471","title":"CLEAR: The Evolution of Spatially Resolved Star Formation in Galaxies between 0.5 ≲ z ≲ 1.7 Using Hα Emission Line Maps","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Saint Mary's University","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Stellar mass; Redshift; Star formation; Galaxy; Reionization; Astronomy; Hubble Ultra-Deep Field; Hubble Deep Field","score_opus":0.014177838240311004,"score_gpt":0.22921293605450727,"score_spread":0.21503509781419627,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296066750","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99870884,0.00005176076,0.00011902925,0.000017987515,0.0000011334186,0.0000020151333,0.0007646791,0.000012893293,0.00032154456],"genre_scores_gemma":[0.9988589,0.000022264308,0.00013742078,0.000005313564,0.0000024550357,0.0000013923384,0.0008123921,0.0000028499728,0.00015689351],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999027,0.000010229231,0.0000040878717,0.000034313744,0.000024532892,0.000024131272],"domain_scores_gemma":[0.99908185,0.0001513371,0.00038593207,0.000043546446,0.0001277187,0.00020968298],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001956967,0.00012950443,0.00012797816,0.0011345267,0.00013673809,0.0006124965,0.0001950795,0.00021193648,0.0010661848],"category_scores_gemma":[0.0010139883,0.00013131148,0.00021016585,0.00056766457,0.0001603243,0.00042612682,0.0004497298,0.00021578105,0.00024858583],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000085520645,0.000020261972,0.98928505,0.000012964496,0.000059191774,0.000065958426,0.00019935734,0.0007500792,0.005476154,0.00014841012,0.00023919939,0.0036579552],"study_design_scores_gemma":[6.0057306e-7,0.000007351013,0.99934477,0.0000012300226,0.0000035585504,0.000017228018,0.000058524583,0.00031446418,0.00014970698,0.000014889842,0.000086318134,0.0000013137526],"about_ca_topic_score_codex":0.010998062,"about_ca_topic_score_gemma":0.01612712,"teacher_disagreement_score":0.010998062,"about_ca_system_score_codex":0.00025982203,"about_ca_system_score_gemma":0.00010189271,"threshold_uncertainty_score":0.02186811},"labels":[],"label_agreement":null},{"id":"W4296280766","doi":"10.3847/1538-4357/ac8b0d","title":"Gastro Library. I. The Simulated Chemodynamical Properties of Several Gaia–Sausage–Enceladus-like Stellar Halos","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Science and Technology Facilities Council; HORIZON EUROPE European Research Council; University of Central Lancashire; National Aeronautics and Space Administration","keywords":"Physics; Halo; Astrophysics; Enceladus; Astrobiology; Astronomy; Galaxy","score_opus":0.008237460507514248,"score_gpt":0.1787562276198451,"score_spread":0.17051876711233085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296280766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9613041,0.0002252736,0.0050241137,0.00043570506,0.00010910946,0.00012774156,0.010757699,0.0067979014,0.015218425],"genre_scores_gemma":[0.980616,0.00012469919,0.0070954966,0.0002158286,0.00005314636,0.00014137023,0.009060862,0.0009508534,0.0017417922],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985576,0.000038654696,0.0000068448967,0.000023021756,0.000032014865,0.000043664626],"domain_scores_gemma":[0.9986873,0.0007471822,0.00011456743,0.00011249657,0.00013044404,0.00020797005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005838021,0.00100408,0.00070285867,0.0008641412,0.0006158286,0.0007843381,0.0020811774,0.0015860164,0.0070399963],"category_scores_gemma":[0.002195882,0.0005659822,0.0011352942,0.0006782913,0.00079790875,0.0005873865,0.0006635044,0.0012549034,0.0008691371],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005713094,0.0004989078,0.025704492,0.00022541967,0.0002644444,0.00048920116,0.00022259829,0.9509311,0.002445276,0.002729362,0.010230869,0.005686985],"study_design_scores_gemma":[0.00023971398,0.00013054704,0.007881464,0.000015447391,0.000034834047,0.00004226851,0.00007390322,0.98881,0.0007708665,0.00063135446,0.0013457999,0.000023823453],"about_ca_topic_score_codex":0.020388005,"about_ca_topic_score_gemma":0.02056923,"teacher_disagreement_score":0.020388005,"about_ca_system_score_codex":0.00094881834,"about_ca_system_score_gemma":0.00075459114,"threshold_uncertainty_score":0.04053867},"labels":[],"label_agreement":null},{"id":"W4296367355","doi":"10.3847/1538-4357/ac86c7","title":"On the Robustness of the Velocity Anisotropy Parameter in Probing the Stellar Kinematics in Milky Way–Like Galaxies: Takeaway from TNG50 Simulation","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Harvard University","keywords":"Physics; Milky Way; Galaxy; Kinematics; Anisotropy; Stellar kinematics; Astrophysics; Robustness (evolution); Astronomy; Classical mechanics; Optics","score_opus":0.018528045479145085,"score_gpt":0.22725616899540116,"score_spread":0.20872812351625608,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296367355","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99698645,0.00016655806,0.0011583418,0.0002311237,0.000025843372,0.000009505033,0.00044216006,0.00019273409,0.0007872454],"genre_scores_gemma":[0.9973571,0.00004698339,0.0010640208,0.00012201147,0.0000141592,0.000011202826,0.0011839491,0.00008540206,0.00011521327],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99918324,0.0004055301,0.000033447126,0.00015891095,0.00007500054,0.00014378854],"domain_scores_gemma":[0.99179345,0.005238669,0.0004586736,0.0011792813,0.0005933968,0.0007366014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0036556288,0.0006375062,0.00075365946,0.000911013,0.000782127,0.0013144711,0.0015836277,0.001279748,0.0008713756],"category_scores_gemma":[0.011377237,0.0003359679,0.0015148037,0.00073912763,0.0010959493,0.0007426038,0.0009168993,0.0010976869,0.00016482576],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010910444,0.0003508279,0.2947708,0.000113492286,0.0010246404,0.00037495288,0.00029284062,0.68415934,0.0050269333,0.0030594573,0.003811053,0.005924542],"study_design_scores_gemma":[0.00020618136,0.00013665055,0.055113558,0.000035114346,0.00018124659,0.00005372103,0.00018254918,0.940479,0.0017523819,0.0011698717,0.0006442391,0.000045528486],"about_ca_topic_score_codex":0.03641321,"about_ca_topic_score_gemma":0.018048476,"teacher_disagreement_score":0.03641321,"about_ca_system_score_codex":0.0008965164,"about_ca_system_score_gemma":0.00058997056,"threshold_uncertainty_score":0.07240254},"labels":[],"label_agreement":null},{"id":"W4296445926","doi":"10.3847/1538-4357/ac8058","title":"CLEAR: The Ionization and Chemical-enrichment Properties of Galaxies at 1.1 &lt; z &lt; 2.3","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Ionization; Galaxy; Astronomy; Ion","score_opus":0.007782014399706022,"score_gpt":0.18634895968390708,"score_spread":0.17856694528420106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296445926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903094,0.00011959852,0.0003062446,0.0001423681,0.0000061665255,0.000008003772,0.006368218,0.00015034112,0.002589702],"genre_scores_gemma":[0.98755276,0.00004623801,0.00043631034,0.000056839348,0.000015259402,0.0000059061726,0.009860219,0.000054878732,0.001971602],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998921,0.0000068150393,0.000004033282,0.000031411368,0.000034373024,0.00003123274],"domain_scores_gemma":[0.99891615,0.00007687918,0.00037032558,0.00009254996,0.00013874078,0.00040536505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037211392,0.00020042736,0.0001609827,0.0012262072,0.00015949072,0.0007359041,0.00025214153,0.00020693307,0.003562089],"category_scores_gemma":[0.00073029246,0.0001711048,0.00016964789,0.00055195676,0.0002296713,0.00054589415,0.0004996336,0.0003514748,0.0010617984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002825516,0.000082021616,0.96804315,0.000024958372,0.000068700196,0.00012538391,0.00036349645,0.000655124,0.010510643,0.00075852853,0.0073020444,0.01178343],"study_design_scores_gemma":[0.0000038825265,0.000008988762,0.99867344,0.000001365536,0.0000038042376,0.000018659372,0.00003075295,0.0002020406,0.00036255733,0.00003904536,0.00065247435,0.0000030488052],"about_ca_topic_score_codex":0.014670512,"about_ca_topic_score_gemma":0.022925835,"teacher_disagreement_score":0.014670512,"about_ca_system_score_codex":0.00036796366,"about_ca_system_score_gemma":0.00014397979,"threshold_uncertainty_score":0.029170275},"labels":[],"label_agreement":null},{"id":"W4296955334","doi":"10.3847/1538-4357/ac8a9e","title":"Accretion Burst Echoes as Probes of Protostellar Environments and Episodic Mass Assembly","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Protostar; Astrophysics; Accretion (finance); Light curve; Amplitude; Envelope (radar); Astronomy; Luminosity; Star formation; Stars; Optics; Galaxy","score_opus":0.007583476780540981,"score_gpt":0.22326566714459775,"score_spread":0.21568219036405678,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4296955334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982967,0.000058421185,0.00053383183,0.000017134209,0.0000029091466,0.0000028841328,0.00018522126,0.000030144693,0.0008728968],"genre_scores_gemma":[0.9993892,0.000013623956,0.0003615264,0.0000058725136,0.000004342369,0.000002072999,0.000117045165,0.0000041072753,0.000102254446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999566,0.000006363445,0.0000025203474,0.00001334126,0.000011074119,0.000010073086],"domain_scores_gemma":[0.99958557,0.00011981853,0.00014445832,0.000040187955,0.000034274675,0.00007566552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022522255,0.00011497536,0.000108898996,0.0006801199,0.0001645111,0.00036509873,0.00015726416,0.0002587674,0.0010237888],"category_scores_gemma":[0.00066835067,0.00011349566,0.00010912363,0.0004172754,0.00011766109,0.00017796848,0.00023148042,0.0001714685,0.00014799177],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002099248,0.000037960177,0.93281776,0.000021549622,0.00003635551,0.00014622486,0.00026550522,0.0014201128,0.053504042,0.00032425567,0.00029279452,0.010923417],"study_design_scores_gemma":[0.000003181355,0.000019296143,0.99542797,0.0000026211299,0.0000052445025,0.0000501326,0.00006108004,0.003015112,0.0011140468,0.00007562098,0.00022260712,0.00000303236],"about_ca_topic_score_codex":0.0017128771,"about_ca_topic_score_gemma":0.0030407668,"teacher_disagreement_score":0.0017128771,"about_ca_system_score_codex":0.00025968606,"about_ca_system_score_gemma":0.0000601896,"threshold_uncertainty_score":0.0034249425},"labels":[],"label_agreement":null},{"id":"W4297415916","doi":"10.3847/1538-4357/ac8981","title":"CLASS: Coronal Line Activity Spectroscopic Survey","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of California, Los Angeles; York University; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; George Mason University; Alfred P. Sloan Foundation; University of Washington; National Science Foundation; Brookhaven National Laboratory; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Princeton University","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Line (geometry); Spectral line; Ionization; Lambda; Accretion (finance); Sky; Geometry","score_opus":0.014236590127508829,"score_gpt":0.23721329061196558,"score_spread":0.22297670048445675,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297415916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8500466,0.00048112957,0.0017778773,0.0001838129,0.000036003734,0.0002464175,0.13250765,0.00074807263,0.0139724985],"genre_scores_gemma":[0.83672714,0.00034718282,0.0032860644,0.00028925558,0.00010377872,0.00024673116,0.14993231,0.00012017585,0.008947335],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99961925,0.00003984888,0.00003690075,0.0001006423,0.00011826035,0.00008512736],"domain_scores_gemma":[0.9980032,0.00008098848,0.0008529219,0.0001832619,0.00045063964,0.00042897812],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043342944,0.00032540265,0.00021306078,0.003509994,0.00031486663,0.0006128095,0.0004899013,0.00024851665,0.008096215],"category_scores_gemma":[0.0009751781,0.00011437645,0.00018604509,0.0016541076,0.000089524256,0.00050354266,0.00068328256,0.00025327806,0.0050002844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009141475,0.00010764769,0.9552634,0.000060407692,0.000039167742,0.00005420444,0.00009683503,0.0001037993,0.004925745,0.00014256746,0.013391174,0.025723675],"study_design_scores_gemma":[0.0000071626464,0.000035004447,0.9892805,0.000010022287,0.000010419661,0.00015541303,0.00007168924,0.00019702184,0.0005711461,0.000058256817,0.009598114,0.0000052349396],"about_ca_topic_score_codex":0.0054094084,"about_ca_topic_score_gemma":0.009252994,"teacher_disagreement_score":0.008096215,"about_ca_system_score_codex":0.0002934786,"about_ca_system_score_gemma":0.0003086831,"threshold_uncertainty_score":0.02708453},"labels":[],"label_agreement":null},{"id":"W4297434854","doi":"10.3847/1538-4357/acdd78","title":"Six More Ultra-faint Milky Way Companions Discovered in the DECam Local Volume Exploration Survey","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; University of Illinois at Urbana-Champaign; Agencia Nacional de Investigación y Desarrollo; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Chinese Academy of Sciences; High Energy Physics; Deutsche Forschungsgemeinschaft; Office of Science; University of Edinburgh; Center for Cosmology and Astroparticle Physics, Ohio State University; University of Sussex; University of Nottingham; University of Cambridge; Kavli Institute for Cosmological Physics, University of Chicago; National Energy Research Scientific Computing Center; National Aeronautics and Space Administration; University College London; Institut de Física d'Altes Energies; Eidgenössische Technische Hochschule Zürich; National Centre for Supercomputing Applications; University of Michigan; Jet Propulsion Laboratory; University of California, Santa Cruz; Ohio State University; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; Financiadora de Estudos e Projetos; University of Pennsylvania; University of Chicago; University of California; California Institute of Technology; U.S. Department of Energy; W. M. Keck Foundation; European Space Agency; Fermilab; Laboratory Directed Research and Development; National Science Foundation; University of Portsmouth; Yale University","keywords":"Physics; Milky Way; Local Group; Astrophysics; Astronomy; Dwarf galaxy; Galaxy; Proper motion; Stars","score_opus":0.028521873938684893,"score_gpt":0.2581343953460283,"score_spread":0.2296125214073434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297434854","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995135,0.00004906421,0.00004634597,0.000010974266,0.0000015351051,0.0000017244497,0.000079338046,0.000004884256,0.00029262935],"genre_scores_gemma":[0.9991755,0.00003013695,0.00014953209,0.00001794117,0.000004644087,0.0000027350823,0.00035320548,0.0000025367149,0.00026366446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979454,0.00001903056,0.0000116379415,0.00006760007,0.000054682318,0.000052510397],"domain_scores_gemma":[0.9991596,0.00008854713,0.0003359106,0.00010247303,0.00007930685,0.00023419497],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027609235,0.00014412196,0.00021161984,0.0013037912,0.00050339487,0.00067910954,0.00031468537,0.00020244652,0.0010137792],"category_scores_gemma":[0.00071018725,0.00012175638,0.000110662244,0.0006949347,0.00030427313,0.0003103583,0.0014545621,0.0001882264,0.00023083529],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000047276022,0.000015340258,0.9910545,0.000008142846,0.000015985366,0.0003691809,0.00040805546,0.000026703083,0.002670767,0.00007996685,0.0002193171,0.005084806],"study_design_scores_gemma":[0.0000063174807,0.000049237085,0.99366295,0.0000068451986,0.000012810303,0.0010734429,0.0006884476,0.00015495776,0.00077732437,0.000051903306,0.0035112302,0.000004458191],"about_ca_topic_score_codex":0.0027777255,"about_ca_topic_score_gemma":0.0073578423,"teacher_disagreement_score":0.0027777255,"about_ca_system_score_codex":0.00024646704,"about_ca_system_score_gemma":0.00013953159,"threshold_uncertainty_score":0.005523145},"labels":[],"label_agreement":null},{"id":"W4297676377","doi":"10.1086/375126","title":"A 3 × 10[TSUP]9[/TSUP] [ITAL]M[/ITAL][TINF]⊙[/TINF] Black Hole in the Quasar SDSS J1148+5251 at [CLC][ITAL]z[/ITAL][/CLC] = 6.41","year":2003,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":270,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Quasar; Physics; Astrophysics; Redshift; Emission spectrum; Luminosity; Spectral line; Equivalent width; Black hole (networking); Eddington luminosity; Infrared; Astronomy; Galaxy","score_opus":0.014559036325161286,"score_gpt":0.23150742380184977,"score_spread":0.2169483874766885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4297676377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97475535,0.00033734104,0.0018467945,0.0015969435,0.0003878691,0.000048059796,0.0014031127,0.00043140282,0.01919319],"genre_scores_gemma":[0.99209154,0.000030346542,0.00045937405,0.00008481066,0.000052987987,0.000005657984,0.0005047913,0.000037357335,0.0067332373],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998504,0.000016496011,0.0000059132226,0.00003905006,0.000034649198,0.00005342445],"domain_scores_gemma":[0.998877,0.0002166318,0.00018531742,0.00008661632,0.00012905398,0.00050541724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003836846,0.0001732259,0.00025338915,0.0005591668,0.00070124085,0.00047874197,0.0003760665,0.00096556044,0.034821387],"category_scores_gemma":[0.0011832758,0.0001229988,0.00037579684,0.00026099067,0.0004432301,0.0005373706,0.00058441615,0.00053064123,0.0018149327],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0039063743,0.0010458068,0.6614754,0.00029994256,0.00020735439,0.009891349,0.001476055,0.002976125,0.036575463,0.042950574,0.14105049,0.098144956],"study_design_scores_gemma":[0.000254626,0.0003665877,0.96433127,0.00004037288,0.00008641719,0.0024573961,0.0012863948,0.0065851035,0.0038011344,0.009644167,0.011085695,0.00006089435],"about_ca_topic_score_codex":0.006458791,"about_ca_topic_score_gemma":0.00621241,"teacher_disagreement_score":0.034821387,"about_ca_system_score_codex":0.00024320063,"about_ca_system_score_gemma":0.0002031866,"threshold_uncertainty_score":0.11648917},"labels":[],"label_agreement":null},{"id":"W4298002547","doi":"10.3847/1538-4357/ac61d9","title":"The Physical Properties of Low-redshift FeLoBAL Quasars. I. Spectral-synthesis Analysis of the Broad Absorption-line (BAL) Outflows Using SimBAL","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Space Agency; Western University","funders":"National Science Foundation","keywords":"Physics; Quasar; Redshift; Astrophysics; Astronomy; Spectral line; Absorption (acoustics); Spectral analysis; Spectroscopy; Optics; Galaxy","score_opus":0.01401807325141015,"score_gpt":0.22495680016351044,"score_spread":0.21093872691210028,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4298002547","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99706656,0.00015551463,0.00087200745,0.000012131947,8.171094e-7,0.000013217344,0.0010193331,0.000038497856,0.0008219242],"genre_scores_gemma":[0.9955264,0.000094537914,0.0013611403,0.000024249448,0.0000035918067,0.000021193751,0.002499945,0.000017520124,0.00045150254],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99976796,0.000050001858,0.000014151353,0.00007605905,0.00005359236,0.000038176233],"domain_scores_gemma":[0.9990625,0.00020933944,0.0003542838,0.000121653546,0.00015228188,0.00009985669],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00070862524,0.0003944282,0.000258032,0.002924185,0.00037491106,0.0006010331,0.00037875667,0.0001805289,0.0011020394],"category_scores_gemma":[0.0010875718,0.00021176015,0.00029848472,0.0011120453,0.00030483934,0.00042951564,0.0009057269,0.00015878589,0.00035600443],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000072709365,0.000028060818,0.97333956,0.00004243507,0.000049187765,0.000062053696,0.00035395965,0.000390146,0.013235862,0.00012971763,0.00018665877,0.012109638],"study_design_scores_gemma":[0.000003831865,0.0000356522,0.9958674,0.0000066813686,0.00001888288,0.000051535433,0.00016013187,0.0008169849,0.0021700675,0.000052647596,0.0008113336,0.000004811056],"about_ca_topic_score_codex":0.005403706,"about_ca_topic_score_gemma":0.0121766785,"teacher_disagreement_score":0.005403706,"about_ca_system_score_codex":0.00040153135,"about_ca_system_score_gemma":0.00012540387,"threshold_uncertainty_score":0.010744512},"labels":[],"label_agreement":null},{"id":"W4298132345","doi":"10.3847/1538-4357/ac7f40","title":"Cleaning Our Hazy Lens: Exploring Trends in Transmission Spectra of Warm Exoplanets","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Japan Society for the Promotion of Science; Heising-Simons Foundation; National Aeronautics and Space Administration","keywords":"Exoplanet; Physics; Planet; Astrophysics; Spectral line; Surface gravity; Astronomy; Stars","score_opus":0.03643545867067448,"score_gpt":0.24218445864468602,"score_spread":0.20574899997401153,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4298132345","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977222,0.00011334928,0.0011343027,0.000021697304,0.0000024410888,0.0000048682878,0.00056197436,0.000067335444,0.00037172905],"genre_scores_gemma":[0.99745196,0.00004176669,0.0013492665,0.0000119141005,0.000008079916,0.000003925636,0.0009811035,0.00002311054,0.00012887099],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997782,0.000035416466,0.000013593641,0.00008360559,0.00005167288,0.000037483023],"domain_scores_gemma":[0.99866986,0.00038567948,0.0004711584,0.000141804,0.00019034377,0.00014111842],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006128547,0.00022659093,0.00028284758,0.0022876891,0.00034123973,0.000543176,0.00029834275,0.000214267,0.0010518468],"category_scores_gemma":[0.001689405,0.00012940125,0.00027604788,0.0015606625,0.00025810188,0.0007297028,0.0006154522,0.0002816842,0.00026661207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010860178,0.000038088616,0.96506727,0.000043077405,0.00014053151,0.00014040772,0.0004100608,0.0010651293,0.015064226,0.000093041424,0.0003537633,0.017475823],"study_design_scores_gemma":[0.0000016052953,0.000022220986,0.9967204,0.0000023681257,0.000014535859,0.00005589451,0.00017373181,0.0012276347,0.0014239766,0.00005036951,0.0003031607,0.0000042839606],"about_ca_topic_score_codex":0.0040688273,"about_ca_topic_score_gemma":0.0056301933,"teacher_disagreement_score":0.0040688273,"about_ca_system_score_codex":0.00023145524,"about_ca_system_score_gemma":0.00012635175,"threshold_uncertainty_score":0.008090258},"labels":[],"label_agreement":null},{"id":"W4298132429","doi":"10.3847/1538-4357/ac8b86","title":"Mapping the Thermal Condensation of Diffuse H i in the North Celestial Pole Loop","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Canadian Institute for Theoretical Astrophysics","keywords":"Physics; Astrophysics; Turbulence; Star formation; Stars; Astronomy; Meteorology","score_opus":0.01703491461779287,"score_gpt":0.223703956831008,"score_spread":0.20666904221321514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4298132429","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984249,0.00003330808,0.00026338347,0.000015185319,0.000001672533,0.0000033953932,0.00021974574,0.000020941256,0.00101755],"genre_scores_gemma":[0.99933547,0.000015004023,0.0002499407,0.0000054621437,0.0000039573465,0.0000024372603,0.000265248,0.0000060559614,0.00011639994],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999149,0.000008642286,0.0000018909524,0.000031953157,0.000021079564,0.000021527798],"domain_scores_gemma":[0.999764,0.0000324387,0.000065935004,0.000027583561,0.00005339472,0.00005659909],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015447897,0.0001394982,0.00013221458,0.0009130273,0.00030271843,0.0004949893,0.0002077135,0.0001477952,0.00096031075],"category_scores_gemma":[0.0004696332,0.0001348555,0.000112001886,0.00072669424,0.0003264224,0.0002577382,0.0004636757,0.0001429801,0.00018232054],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007377618,0.00008598243,0.859663,0.0000391787,0.000055930574,0.000219455,0.0011428286,0.0031626842,0.10830906,0.0008031579,0.0006959644,0.025084965],"study_design_scores_gemma":[0.000008308709,0.00002142114,0.99427515,0.0000030284323,0.000006127288,0.000022426095,0.00011934281,0.0028022623,0.0019257171,0.00008572322,0.0007260094,0.000004495908],"about_ca_topic_score_codex":0.023002636,"about_ca_topic_score_gemma":0.02960102,"teacher_disagreement_score":0.023002636,"about_ca_system_score_codex":0.00063931633,"about_ca_system_score_gemma":0.00019418536,"threshold_uncertainty_score":0.045737445},"labels":[],"label_agreement":null},{"id":"W4298132440","doi":"10.3847/1538-4357/ac898f","title":"Changes in the Na D<sub>1</sub> Absorption Components of η Carinae Provide Clues on the Location of the Dissipating Central Occulter","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Space Telescope Science Institute","keywords":"Physics; Astrophysics; Absorption (acoustics); Spectral line; Absorption spectroscopy; Astronomy; Ionization; Stars; Ultraviolet; Optics; Ion","score_opus":0.01725144136941613,"score_gpt":0.234106002687145,"score_spread":0.21685456131772884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4298132440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99685836,0.00010753636,0.00021366039,0.000020043006,0.000003749588,0.0000026601192,0.0001807142,0.000027117823,0.0025860493],"genre_scores_gemma":[0.99902344,0.00003288092,0.00019894798,0.000011812816,0.0000022778017,0.0000016575503,0.00019501793,0.0000059209106,0.00052806863],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999664,0.0000017056472,0.0000012086293,0.000012287373,0.000008470799,0.000010004244],"domain_scores_gemma":[0.9998951,0.000011941187,0.000028982999,0.000007963623,0.000027621452,0.000028368042],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006995918,0.00011917167,0.000090219975,0.00064251764,0.00036407862,0.00029818865,0.00016689036,0.0002071121,0.002499589],"category_scores_gemma":[0.00014278146,0.00009798684,0.000077533594,0.0002757627,0.00015765785,0.00021232704,0.00018149042,0.00021231167,0.0004609496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015949811,0.000042770112,0.7543427,0.000042440144,0.00002823556,0.00024382077,0.0005049702,0.00020942792,0.22889444,0.00020339123,0.00052810035,0.0148002915],"study_design_scores_gemma":[6.5860854e-7,0.0000097618695,0.99563295,0.0000023135492,0.000003037367,0.000051964114,0.000131305,0.00022348561,0.0031412328,0.000013702,0.00078809384,0.0000016042429],"about_ca_topic_score_codex":0.0053374935,"about_ca_topic_score_gemma":0.015909117,"teacher_disagreement_score":0.0053374935,"about_ca_system_score_codex":0.00029769124,"about_ca_system_score_gemma":0.000061353254,"threshold_uncertainty_score":0.010612905},"labels":[],"label_agreement":null},{"id":"W4298132486","doi":"10.3847/1538-4357/ac90c0","title":"Errors When Constraining Hot Blackbody Parameters with Optical Photometry","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"European Research Council; Israel Science Foundation; United States - Israel Binational Science Foundation","keywords":"Black-body radiation; Physics; Photometry (optics); Prior probability; Astrophysics; Optical depth; Optics; Statistics; Radiation; Bayesian probability; Stars; Mathematics","score_opus":0.01563251223695714,"score_gpt":0.22890472420259128,"score_spread":0.21327221196563415,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4298132486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8754681,0.0005349518,0.11607508,0.00039278314,0.00008062358,0.000042563668,0.00093684165,0.0011388798,0.0053301314],"genre_scores_gemma":[0.9883754,0.00006212086,0.010326581,0.000121681376,0.000014547758,0.000022451186,0.0005955779,0.00019210468,0.0002895769],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99833715,0.000778423,0.00008232146,0.0003868275,0.00028543442,0.00012986863],"domain_scores_gemma":[0.99168617,0.0049780146,0.00087192294,0.0017580804,0.0004994587,0.00020624208],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004465422,0.0007244218,0.00041323574,0.0006499807,0.00061828457,0.0012219114,0.0011663856,0.0006161022,0.0014060228],"category_scores_gemma":[0.014044902,0.0006050166,0.000791822,0.0007950409,0.001263587,0.0016171286,0.0011937533,0.0007319106,0.0003481245],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041239095,0.00010625666,0.30440947,0.00012200966,0.00036617334,0.00015430336,0.0004296835,0.6489929,0.007823321,0.010029151,0.001492452,0.02566199],"study_design_scores_gemma":[0.0001058711,0.0001208846,0.12996201,0.00020043689,0.00016549145,0.00021025687,0.00034457518,0.81134117,0.024625562,0.024409154,0.008389763,0.0001248596],"about_ca_topic_score_codex":0.0064758873,"about_ca_topic_score_gemma":0.0057591023,"teacher_disagreement_score":0.0064758873,"about_ca_system_score_codex":0.0008588138,"about_ca_system_score_gemma":0.00040688599,"threshold_uncertainty_score":0.023615658},"labels":[],"label_agreement":null},{"id":"W4300621309","doi":"10.1086/308284","title":"The Luminous Type Ic Supernova 1992ar at \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $z=0.145$ \\end{document}","year":2000,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dominion Astrophysical Observatory","funders":"","keywords":"Physics; Supernova; Redshift; Astrophysics; Type (biology); Photometry (optics); Spectral line; Universe; Galaxy; Astronomy; Stars","score_opus":0.011430005454003923,"score_gpt":0.24122981712735647,"score_spread":0.22979981167335256,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4300621309","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.038538497,0.0009258362,0.0066836025,0.0012952808,0.00153909,0.00036809768,0.082956016,0.017370136,0.8503235],"genre_scores_gemma":[0.085938856,0.0013268436,0.0066439114,0.000485007,0.00043447025,0.00009746369,0.10135476,0.009307389,0.79441124],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99987924,0.0000062487193,0.0000053321664,0.000026639076,0.00006400159,0.000018473815],"domain_scores_gemma":[0.9996928,0.000046441364,0.0000448885,0.000072955445,0.000093931776,0.000049004026],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.000111886184,0.000330433,0.00013775562,0.00088478427,0.0004158651,0.0019357216,0.00045275627,0.0003536381,0.29002488],"category_scores_gemma":[0.0008295046,0.00017518643,0.00024383981,0.0011519091,0.00016695655,0.0006749539,0.000413052,0.00043428593,0.17624679],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015632385,0.00007414389,0.004474323,0.00037589605,0.000010505977,0.00027424077,0.000123014,0.00028058357,0.008507007,0.0042293086,0.8492393,0.13225546],"study_design_scores_gemma":[0.000022891722,0.000025242134,0.015718352,0.000063184496,0.000008491686,0.00023656874,0.000043544052,0.00028361948,0.0035989082,0.00041670838,0.9795751,0.000007423283],"about_ca_topic_score_codex":0.010095179,"about_ca_topic_score_gemma":0.016680293,"teacher_disagreement_score":0.7099751,"about_ca_system_score_codex":0.00069895404,"about_ca_system_score_gemma":0.0003838456,"threshold_uncertainty_score":0.97022986},"labels":[],"label_agreement":null},{"id":"W4300629138","doi":"10.1086/508138","title":"Multiwavelength Mass Comparisons of the \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $z\\sim 0.3$ \\end{document} CNOC Cluster Sample","year":2006,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of Toronto; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Hydrostatic equilibrium; Galaxy cluster; Surface brightness; Redshift; Cosmology; Galaxy; Scaling; Spectral line; Geometry; Quantum mechanics; Mathematics","score_opus":0.009863168412018503,"score_gpt":0.22905868747421151,"score_spread":0.219195519062193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4300629138","genre_codex":"empirical","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.912241,0.00020838728,0.0010663086,0.00008733816,0.000014473952,0.00009298198,0.032763924,0.0005413961,0.052984264],"genre_scores_gemma":[0.90989345,0.00019501214,0.0031077657,0.000043820124,0.0000091797065,0.0000468255,0.03916072,0.00032420587,0.047218986],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.99985313,0.000004991542,0.0000075697,0.00004177032,0.000058751422,0.00003372073],"domain_scores_gemma":[0.99962604,0.000048891012,0.000050861014,0.00006474957,0.00012850684,0.000080943515],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00019014337,0.000163041,0.0001121959,0.001586536,0.00036504184,0.00046571356,0.0004837534,0.00011457708,0.021309428],"category_scores_gemma":[0.00060314976,0.000092025744,0.00018262553,0.001448745,0.00012081658,0.0003088423,0.00050069176,0.00011754178,0.0035716407],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018306915,0.00030806483,0.58467215,0.0002794045,0.000119928016,0.00043311145,0.0032092675,0.0031655624,0.052919712,0.0060016364,0.079164565,0.26789588],"study_design_scores_gemma":[0.0000137018,0.000037568345,0.9697986,0.000009873791,0.000025015413,0.000056558238,0.0003825871,0.0009160246,0.005247213,0.00014180092,0.023359353,0.000011665655],"about_ca_topic_score_codex":0.2038751,"about_ca_topic_score_gemma":0.4142731,"teacher_disagreement_score":0.97869056,"about_ca_system_score_codex":0.0013755844,"about_ca_system_score_gemma":0.0006738157,"threshold_uncertainty_score":0.4053768},"labels":[],"label_agreement":null},{"id":"W4300660872","doi":"10.1086/587449","title":"The Nascent Red Sequence at \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $z\\sim 2$ \\end{document}","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":74,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Astrophysics; Galaxy; Redshift; Star formation; Galaxy formation and evolution; Population; Radio galaxy; Astronomy; Medicine","score_opus":0.017750042194897012,"score_gpt":0.24352383563786797,"score_spread":0.22577379344297097,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4300660872","genre_codex":"other","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":"other","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00202564,0.0003883641,0.045444883,0.0011645869,0.0023425084,0.0009926682,0.1329381,0.16970614,0.6449971],"genre_scores_gemma":[0.008641726,0.00052608224,0.013774663,0.0008590126,0.00054004684,0.00039772395,0.096103474,0.12782617,0.75133103],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99952865,0.000041189676,0.000033280026,0.00010302602,0.00020165108,0.00009228976],"domain_scores_gemma":[0.99754167,0.0004327826,0.00011122098,0.000890573,0.00076435413,0.00025944455],"candidate_categories":["insufficient_payload"],"consensus_categories":["insufficient_payload"],"category_scores_codex":[0.00068907905,0.0024037529,0.0010371177,0.0018592302,0.0013912673,0.0065831016,0.0024557028,0.001810118,0.84335625],"category_scores_gemma":[0.004027421,0.001561819,0.0016100467,0.0020400118,0.00063232094,0.004286498,0.0029825708,0.002683991,0.8644859],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016380702,0.00005512895,0.00030933344,0.0002819187,0.000010576998,0.000060100883,0.00010009084,0.00017239295,0.0019238171,0.0042265086,0.9475255,0.045170736],"study_design_scores_gemma":[0.000030006417,0.000016549275,0.00041766715,0.00005784015,0.0000056644576,0.000070876835,0.000028257564,0.00021169987,0.0020641743,0.000908215,0.9961731,0.000016075926],"about_ca_topic_score_codex":0.0074639064,"about_ca_topic_score_gemma":0.0059361258,"teacher_disagreement_score":0.15664375,"about_ca_system_score_codex":0.002230649,"about_ca_system_score_gemma":0.0010173954,"threshold_uncertainty_score":0.2234332},"labels":[],"label_agreement":null},{"id":"W4300960963","doi":"10.3847/1538-4357/ac8cfe","title":"Establishing Dust Rings and Forming Planets within Them","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Fonds de recherche du Québec – Nature et technologies","keywords":"Physics; Planetesimal; Planet; Astrophysics; Interplanetary dust cloud; Cosmic dust; Accretion (finance); Dust lane; Astronomy; Gas giant; Solar System; Star formation; Stars; Exoplanet","score_opus":0.013667959187076495,"score_gpt":0.21663422764476314,"score_spread":0.20296626845768664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4300960963","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99723107,0.000054752294,0.0010613165,0.00004016501,0.000009394469,0.00000829437,0.00003973446,0.000030323174,0.0015249399],"genre_scores_gemma":[0.9987796,0.000035339446,0.0008058957,0.000011641037,0.0000029856342,0.0000038100377,0.000048335325,0.000010623229,0.00030169706],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999039,0.000018444502,0.000004014457,0.000028654933,0.0000133197345,0.000031603802],"domain_scores_gemma":[0.9995889,0.00010489715,0.00007330939,0.000054194425,0.000026453192,0.00015223342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035126694,0.00017372312,0.00029624786,0.00024976727,0.0006799491,0.0011990686,0.00049030135,0.0004638775,0.0025093309],"category_scores_gemma":[0.0011520545,0.00026112658,0.0002951757,0.00014027157,0.0008015553,0.00089128764,0.00081324496,0.00038358587,0.00021907914],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005582522,0.00027064697,0.18464743,0.00017206829,0.00019598207,0.0011095159,0.0010465628,0.7362672,0.044451226,0.020826895,0.0013243837,0.009129794],"study_design_scores_gemma":[0.00017901581,0.00046359896,0.06729426,0.000045090816,0.00009169491,0.00030861812,0.00088571693,0.90908587,0.009212889,0.007257782,0.005115871,0.00005957178],"about_ca_topic_score_codex":0.004476403,"about_ca_topic_score_gemma":0.0033289932,"teacher_disagreement_score":0.004476403,"about_ca_system_score_codex":0.0005094162,"about_ca_system_score_gemma":0.00036033025,"threshold_uncertainty_score":0.008900702},"labels":[],"label_agreement":null},{"id":"W4300961028","doi":"10.3847/1538-4357/ac8c27","title":"SDSS-IV MaNGA: Unveiling Galaxy Interaction by Merger Stages with Machine Learning","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; Natural Sciences and Engineering Research Council of Canada; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Chung-Hsing University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Galaxy; Astrophysics; Sky; Line-of-sight; Active galactic nucleus; Galaxy merger; Star formation; Astronomy","score_opus":0.0057235647369018915,"score_gpt":0.20897106004799326,"score_spread":0.20324749531109138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4300961028","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9757523,0.0006866828,0.013131789,0.00025373272,0.000033628185,0.000062999046,0.0053386227,0.0025288202,0.0022113968],"genre_scores_gemma":[0.97333354,0.000050651754,0.017297253,0.00006200528,0.000037446764,0.000035644553,0.008495234,0.0001292587,0.0005589441],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993592,0.00023854306,0.000033987926,0.00015848652,0.00010818886,0.00010171694],"domain_scores_gemma":[0.9981482,0.00072227896,0.00034151264,0.0003223967,0.00021534618,0.00025033488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015473879,0.0006710636,0.0005234862,0.003476978,0.0004621265,0.0008490996,0.0005932135,0.00044371941,0.0010002842],"category_scores_gemma":[0.0027680078,0.00023243584,0.0007049913,0.0015732537,0.0002795095,0.00062216347,0.00086666737,0.00057406153,0.0008967688],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004529189,0.0002471797,0.8566051,0.000095916264,0.0004261606,0.00013927667,0.00017277875,0.027778912,0.010500444,0.0006054113,0.007725442,0.09525041],"study_design_scores_gemma":[0.000039535666,0.000116085925,0.60411376,0.000024514542,0.00006865759,0.00007347447,0.00019262936,0.38513443,0.00535238,0.0011839595,0.003657995,0.000042590644],"about_ca_topic_score_codex":0.0068762256,"about_ca_topic_score_gemma":0.008819571,"teacher_disagreement_score":0.0068762256,"about_ca_system_score_codex":0.00048374923,"about_ca_system_score_gemma":0.00030608723,"threshold_uncertainty_score":0.013672411},"labels":[],"label_agreement":null},{"id":"W4301395365","doi":"10.3847/1538-4357/ac905c","title":"A Millimeter-multiwavelength Continuum Study of VLA 1623 West","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Millimeter; Astrophysics; Protoplanetary disk; Circumstellar disk; Wavelength; Planet; Submillimeter Array; Debris disk; Astronomy; Thick disk; Accretion disc; Planetary system; Stars; Star formation; Galaxy; Optics; Halo","score_opus":0.012761698198755129,"score_gpt":0.2424546208478574,"score_spread":0.22969292264910227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4301395365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99921393,0.000022902383,0.00016482438,0.000020153386,0.0000017210991,0.000003846194,0.00016397836,0.000014819402,0.00039395792],"genre_scores_gemma":[0.9988154,0.000019142404,0.00029863312,0.000033007364,0.0000051130287,0.0000051465595,0.00042639405,0.000011320105,0.00038591764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999354,0.000009851158,0.0000032586547,0.000021398935,0.000014007569,0.000016075968],"domain_scores_gemma":[0.9997311,0.000030613082,0.00009814505,0.000020981055,0.00002056769,0.00009839556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019569857,0.0003163184,0.00025791442,0.00054992066,0.0005613434,0.00040253336,0.00025722952,0.00037822122,0.0010910472],"category_scores_gemma":[0.000250104,0.00019151949,0.00025370775,0.00052537775,0.00021802243,0.00022038876,0.00030417537,0.0003786621,0.0005073439],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037603464,0.0006860928,0.9204324,0.00004057647,0.00008058429,0.0031865034,0.0014202942,0.0007733653,0.06115957,0.00046020775,0.0011209466,0.010263421],"study_design_scores_gemma":[0.0000069377556,0.00008091145,0.997168,0.0000038331136,0.000009174989,0.00056188105,0.00026435335,0.0008388983,0.0005928956,0.000053530533,0.00041577118,0.0000037435805],"about_ca_topic_score_codex":0.009585221,"about_ca_topic_score_gemma":0.01582128,"teacher_disagreement_score":0.009585221,"about_ca_system_score_codex":0.00037591028,"about_ca_system_score_gemma":0.00013527084,"threshold_uncertainty_score":0.019058883},"labels":[],"label_agreement":null},{"id":"W4301603182","doi":"10.3847/1538-4357/ac8f27","title":"The Expansion of the X-Ray Nebula Around η Car","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Astrophysics Science Division; Natural Sciences and Engineering Research Council of Canada; Goddard Space Flight Center; Nuclear Safety and Security Commission; Space Telescope Science Institute; Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration","keywords":"Physics; Ejecta; Astrophysics; Nebula; Acis; X-ray; Light curve; Astronomy; Shock wave; Flux (metallurgy); Kinetic energy; Supernova; Stars; Optics","score_opus":0.0112660085996508,"score_gpt":0.22149081288425035,"score_spread":0.21022480428459955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4301603182","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99882036,0.000058271333,0.00008668206,0.000006953839,0.0000013588954,0.0000015731624,0.00003483654,0.000007417375,0.00098254],"genre_scores_gemma":[0.9996575,0.000022445973,0.00007624025,0.0000032339665,0.000001617854,7.853055e-7,0.00006395019,0.0000016771294,0.00017252953],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995184,0.0000040543946,0.0000013855798,0.000018872182,0.0000121291005,0.000011657136],"domain_scores_gemma":[0.9998405,0.000029187779,0.000042647524,0.000016481083,0.00003522562,0.000035901176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014273409,0.000083852145,0.00008545196,0.0004421251,0.00032532975,0.0004139073,0.00019099445,0.00010198826,0.0008445796],"category_scores_gemma":[0.0002866526,0.00008243849,0.000088644774,0.00016204843,0.0002289125,0.00018638298,0.000300916,0.00016479212,0.00016599652],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017543229,0.00004227906,0.8975541,0.000046292356,0.00006303708,0.0004462513,0.00045870928,0.0019745773,0.08812572,0.00072162005,0.00027525928,0.0101167355],"study_design_scores_gemma":[0.0000029659516,0.000042883265,0.9938212,0.000006220285,0.000013366483,0.00015613601,0.00010467671,0.0022334247,0.00259806,0.000041541654,0.00097618985,0.000003365187],"about_ca_topic_score_codex":0.008015959,"about_ca_topic_score_gemma":0.009853987,"teacher_disagreement_score":0.008015959,"about_ca_system_score_codex":0.0003821957,"about_ca_system_score_gemma":0.00015332435,"threshold_uncertainty_score":0.01593858},"labels":[],"label_agreement":null},{"id":"W4302613704","doi":"10.1086/522879","title":"A Multiwavelength Analysis of the Strong Lensing Cluster RCS 022434‐0002.5 at \\documentclass{aastex} \\usepackage{amsbsy} \\usepackage{amsfonts} \\usepackage{amssymb} \\usepackage{bm} \\usepackage{mathrsfs} \\usepackage{pifont} \\usepackage{stmaryrd} \\usepackage{textcomp} \\usepackage{portland,xspace} \\usepackage{amsmath,amsxtra} \\usepackage[OT2,OT1]{fontenc} \\newcommand\\cyr{ \\renewcommand\\rmdefault{wncyr} \\renewcommand\\sfdefault{wncyss} \\renewcommand\\encodingdefault{OT2} \\normalfont \\selectfont} \\DeclareTextFontCommand{\\textcyr}{\\cyr} \\pagestyle{empty} \\DeclareMathSizes{10}{9}{7}{6} \\begin{document} \\landscape $z=0.778$ \\end{document}","year":2007,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto; University of Victoria","funders":"","keywords":"Physics; Astrophysics; Cluster (spacecraft); Redshift; Surface brightness; RADIUS; Velocity dispersion; Galaxy","score_opus":0.014062551509777076,"score_gpt":0.26296400054976227,"score_spread":0.24890144903998518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4302613704","genre_codex":"empirical","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98746663,0.00013632157,0.00045699102,0.00013509428,0.00001321393,0.000024305527,0.0020882098,0.00035795826,0.009321328],"genre_scores_gemma":[0.98779464,0.00009426365,0.0012786747,0.000057029967,0.000021551878,0.000022809127,0.004559053,0.00019181593,0.0059802304],"study_design_codex":"bench_or_experimental","study_design_gemma":"not_applicable","domain_scores_codex":[0.9998859,0.0000053041044,0.0000040523378,0.000026956868,0.000044210417,0.000033502838],"domain_scores_gemma":[0.99970263,0.000035823756,0.00005795448,0.000036421607,0.00004526617,0.000121862286],"candidate_categories":["insufficient_payload"],"consensus_categories":[],"category_scores_codex":[0.00010363114,0.00035678674,0.00029231358,0.001156316,0.00052288454,0.00046267477,0.0005154985,0.00029130478,0.0061104586],"category_scores_gemma":[0.00024019313,0.00022860648,0.0003667785,0.0010661788,0.00018181432,0.00015130054,0.000444578,0.00035761273,0.0018449804],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019836642,0.0005011692,0.3213298,0.0004910513,0.00037882334,0.004329497,0.0017674516,0.015847625,0.5574371,0.0032683348,0.03322373,0.05944175],"study_design_scores_gemma":[0.000041675714,0.00009398451,0.9709173,0.000015592246,0.00006724512,0.00028215593,0.0003226692,0.006170351,0.014389733,0.0001967511,0.007467738,0.000034772245],"about_ca_topic_score_codex":0.019459883,"about_ca_topic_score_gemma":0.031309757,"teacher_disagreement_score":0.9938896,"about_ca_system_score_codex":0.0007667683,"about_ca_system_score_gemma":0.0003322145,"threshold_uncertainty_score":0.03869319},"labels":[],"label_agreement":null},{"id":"W4304194086","doi":"10.3847/1538-4357/ac8ea7","title":"High-Cadence TESS and Ground-based Data of SN 2019esa, the Less Energetic Sibling of SN 2006gy <sup>∗</sup>","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"National Aeronautics and Space Administration; Heising-Simons Foundation; National Science Foundation","keywords":"Light curve; Physics; Astrophysics; Luminosity; Supernova; Spectral line; Emission spectrum; Stars; Astronomy; Galaxy","score_opus":0.025750443004958278,"score_gpt":0.24486032147758183,"score_spread":0.21910987847262356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304194086","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99133897,0.000045677032,0.00023045053,0.000025512794,0.000007897098,0.0000072411335,0.006076797,0.00005894716,0.0022085842],"genre_scores_gemma":[0.97440195,0.000036428723,0.00076876045,0.000025462727,0.000018944338,0.000007879429,0.023570666,0.000023360319,0.0011464229],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999162,0.0000057321613,0.000007793954,0.000023308627,0.00002712865,0.000019798024],"domain_scores_gemma":[0.99952686,0.000035662204,0.00013497025,0.00006678289,0.00009290031,0.00014275592],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017961787,0.0001666836,0.00017208896,0.0010838154,0.00028306933,0.00033970978,0.00017021988,0.00019839482,0.0019795217],"category_scores_gemma":[0.0002990593,0.000095004,0.00020499047,0.0007734277,0.00014032683,0.00018857149,0.0003917287,0.00014421063,0.00095412246],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001069165,0.00021146686,0.9113224,0.00006151765,0.00008937536,0.0011392924,0.00024712656,0.00090731494,0.059942883,0.00036576425,0.0036862053,0.020957474],"study_design_scores_gemma":[0.0000058774494,0.000055198707,0.99430966,0.000002571495,0.0000107313135,0.00040370607,0.00006563616,0.0003848731,0.0019770472,0.000041316107,0.0027392125,0.0000040452514],"about_ca_topic_score_codex":0.0046838406,"about_ca_topic_score_gemma":0.011494472,"teacher_disagreement_score":0.0046838406,"about_ca_system_score_codex":0.00025985102,"about_ca_system_score_gemma":0.00011900202,"threshold_uncertainty_score":0.009313166},"labels":[],"label_agreement":null},{"id":"W4304694332","doi":"10.3847/1538-4357/ac8b7b","title":"X-Ray Polarization Detection of Cassiopeia A with IXPE","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Horizon 2020 Framework Programme","keywords":"Physics; Polarization (electrochemistry); Cassiopeia A; Astrophysics; Magnetic field; Polarimetry; Synchrotron radiation; Supernova remnant; Spectral index; Degree of polarization; Circular polarization; Supernova; Optics; Scattering; Astronomy; Spectral line","score_opus":0.004983261470508446,"score_gpt":0.19233364044415913,"score_spread":0.18735037897365067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304694332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99492955,0.00015485208,0.0008663131,0.00007351459,0.00001423336,0.00001557488,0.00061016926,0.0000760196,0.0032597722],"genre_scores_gemma":[0.9977126,0.00008019154,0.0010199678,0.000043942593,0.000022672448,0.000010165152,0.0008016344,0.000013815341,0.00029495574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996791,0.000029340825,0.00001297452,0.00013196075,0.000084424355,0.00006224397],"domain_scores_gemma":[0.9992017,0.00013828435,0.00023257491,0.00014703904,0.00013803913,0.00014230027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000461726,0.00043140075,0.00024468452,0.0008518971,0.0006260411,0.00085147226,0.00028401116,0.00047236943,0.0012856236],"category_scores_gemma":[0.00086850463,0.00028156978,0.0003263085,0.00056866533,0.00042414808,0.00023573427,0.0009384906,0.0004871861,0.0003503459],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008764108,0.0001175157,0.7043292,0.00010497826,0.00026532725,0.0022630175,0.00041396366,0.0005812106,0.27382964,0.00073496747,0.001499107,0.014984688],"study_design_scores_gemma":[0.000033543784,0.0002657745,0.9472336,0.000022320295,0.00008253718,0.002174981,0.00015484124,0.0014301052,0.043051377,0.0002692209,0.0052597993,0.000021963],"about_ca_topic_score_codex":0.0011193607,"about_ca_topic_score_gemma":0.0010464725,"teacher_disagreement_score":0.0012856236,"about_ca_system_score_codex":0.00018791136,"about_ca_system_score_gemma":0.00014949647,"threshold_uncertainty_score":0.004300773},"labels":[],"label_agreement":null},{"id":"W4304694493","doi":"10.3847/1538-4357/ac8de4","title":"Search for Astrophysical Neutrinos from 1FLE Blazars with IceCube","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Natural Sciences and Engineering Research Council of Canada; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; University of Oxford; Compute Canada; Marquette University; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; U.S. Department of Energy; Vetenskapsrådet","keywords":"Physics; Blazar; Neutrino; Astrophysics; Neutrino detector; Neutrino astronomy; Muon; Fermi Gamma-ray Space Telescope; Flux (metallurgy); Muon neutrino; Astronomy; Particle physics; Gamma ray; Neutrino oscillation","score_opus":0.011456229985311745,"score_gpt":0.22997392831812946,"score_spread":0.21851769833281773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304694493","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96590334,0.000730996,0.0027301563,0.0002060043,0.00003831771,0.000072846946,0.017954629,0.0004189123,0.011944711],"genre_scores_gemma":[0.9424427,0.00033504463,0.005664881,0.00016491994,0.00006218587,0.00009431591,0.04840243,0.000095693336,0.0027378243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994529,0.00006050043,0.000021950016,0.00016774853,0.0001603404,0.00013658071],"domain_scores_gemma":[0.9984939,0.00032330994,0.0005968497,0.00016021008,0.00025674186,0.0001689777],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013987882,0.0004481866,0.0005039796,0.002755351,0.0006857599,0.0014192638,0.00035857782,0.0004321235,0.0032951604],"category_scores_gemma":[0.0014956603,0.00021931884,0.00042213005,0.0019430842,0.00023737035,0.0005329288,0.0007832029,0.00040349193,0.0006198127],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006823502,0.00018334985,0.9312212,0.0001033648,0.00030957776,0.00048145922,0.0003375423,0.0022198805,0.019934189,0.0010252129,0.0072956574,0.036206152],"study_design_scores_gemma":[0.00003511464,0.00010940302,0.96848387,0.000035369605,0.000078454286,0.00027458367,0.00016383869,0.003004857,0.0078037195,0.0003202884,0.019673675,0.000016940623],"about_ca_topic_score_codex":0.012960036,"about_ca_topic_score_gemma":0.02338561,"teacher_disagreement_score":0.012960036,"about_ca_system_score_codex":0.001015657,"about_ca_system_score_gemma":0.00062014826,"threshold_uncertainty_score":0.025769234},"labels":[],"label_agreement":null},{"id":"W4304694592","doi":"10.3847/1538-4357/ac8b08","title":"The Role of Binarity and Stellar Rotation in the Split Main Sequence of NGC 2422","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Stars; Photometry (optics); Stellar rotation; Astronomy; Star cluster; Stellar classification","score_opus":0.010744117992014475,"score_gpt":0.22596073564741104,"score_spread":0.21521661765539657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304694592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99936444,0.000040346014,0.00012955695,0.000016028944,0.0000017382857,0.0000011136206,0.00009287512,0.000010593564,0.0003433641],"genre_scores_gemma":[0.99974805,0.0000071204995,0.000052549734,0.0000028996526,0.0000016040517,0.0000011041184,0.00012641541,0.000005906824,0.00005428634],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996643,0.00008384813,0.000021438616,0.00011003188,0.00006219108,0.000058139973],"domain_scores_gemma":[0.997551,0.00072533474,0.0006215238,0.00031673812,0.00028936806,0.0004959627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067408103,0.00020912402,0.00035372277,0.0011612179,0.0006038412,0.0010339549,0.0003164749,0.0002874161,0.001779948],"category_scores_gemma":[0.0031761983,0.00014681632,0.00015855319,0.0006984387,0.00056882174,0.0003301729,0.00049672177,0.0001731879,0.00043266013],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002391482,0.00002052246,0.98624295,0.000008230459,0.000051935764,0.0001578102,0.00033674395,0.0017876663,0.006313332,0.00038711005,0.00019982723,0.00425459],"study_design_scores_gemma":[0.000004091269,0.000020183887,0.9949556,0.0000036011722,0.000010773428,0.00007491225,0.00013718224,0.0039134393,0.00039993323,0.0002688348,0.00020389826,0.000007492057],"about_ca_topic_score_codex":0.013165258,"about_ca_topic_score_gemma":0.018359622,"teacher_disagreement_score":0.013165258,"about_ca_system_score_codex":0.00069525925,"about_ca_system_score_gemma":0.00023351025,"threshold_uncertainty_score":0.026177287},"labels":[],"label_agreement":null},{"id":"W4304808898","doi":"10.3847/1538-4357/ac8f41","title":"Searching for Supernova Bursts in Super-Kamiokande IV","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg; British Columbia Institute of Technology; TRIUMF; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Supernova; Physics; Astrophysics; Neutrino; Limit (mathematics); Super-Kamiokande; Event (particle physics); Core (optical fiber); Astronomy; Nuclear physics; Neutrino oscillation; Solar neutrino; Optics; Mathematics","score_opus":0.024627817417904572,"score_gpt":0.30649493878324224,"score_spread":0.28186712136533765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304808898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986041,0.00007380587,0.00019257463,0.000009829274,0.0000029842615,0.00000645466,0.00035154913,0.000008206254,0.0007505056],"genre_scores_gemma":[0.9977385,0.000082038925,0.0003658747,0.000010071716,0.000004205012,0.000009663916,0.0013048651,0.0000044373764,0.00048045669],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980587,0.00002175749,0.000016643384,0.0000626766,0.00004794458,0.000045120203],"domain_scores_gemma":[0.9991084,0.00014965728,0.00033021282,0.00009539269,0.00013482038,0.00018154786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004125007,0.00022468335,0.0002662003,0.002172732,0.00026805492,0.0006996061,0.00029991785,0.00021123886,0.0009373897],"category_scores_gemma":[0.0007119187,0.00016291883,0.0002620224,0.0013399522,0.00023301807,0.00040507223,0.00076277135,0.0002860536,0.00027544162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021723722,0.000056650475,0.9801703,0.000041705844,0.000108731525,0.0005699486,0.00030274806,0.00038263877,0.010627083,0.00020027073,0.00015820554,0.007164509],"study_design_scores_gemma":[0.0000060214747,0.00007924184,0.9953431,0.000013281076,0.000031852593,0.0002504316,0.000320273,0.0005052411,0.0018373422,0.00013643222,0.0014694126,0.000007420772],"about_ca_topic_score_codex":0.0028675662,"about_ca_topic_score_gemma":0.0040532444,"teacher_disagreement_score":0.0028675662,"about_ca_system_score_codex":0.00021735534,"about_ca_system_score_gemma":0.0002584284,"threshold_uncertainty_score":0.0057017803},"labels":[],"label_agreement":null},{"id":"W4304889397","doi":"10.3847/1538-4357/ac8ff0","title":"Protostellar and Protoplanetary Disk Masses in the Serpens Region","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Science Foundation","keywords":"Serpens; Ophiuchus; Protostar; Physics; Astrophysics; Millimeter; Star formation; Submillimeter Array; Young stellar object; Astronomy; Molecular cloud; Stars","score_opus":0.011919839096396878,"score_gpt":0.22393823140735072,"score_spread":0.21201839231095385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304889397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993412,0.000075453994,0.00002951965,0.000004144749,0.0000011214172,0.0000011753338,0.00013833768,0.0000031817528,0.00040585597],"genre_scores_gemma":[0.99946636,0.00007809674,0.00005267404,0.000004213672,0.0000016092067,0.0000010209521,0.00022617963,0.0000018246948,0.00016796128],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991035,0.000013467899,0.000009275069,0.000028573579,0.000016066217,0.000022238191],"domain_scores_gemma":[0.9996227,0.000046013403,0.00018267357,0.000041972224,0.000031981373,0.00007468564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015734503,0.0002206764,0.00018337881,0.001042677,0.000166665,0.00048372592,0.00014994145,0.00010906329,0.0013323589],"category_scores_gemma":[0.00057626504,0.00008805092,0.00016742287,0.0004443446,0.00029954864,0.0002455387,0.00041510878,0.0000908866,0.00031627403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000162303,0.000015910877,0.98680335,0.000025211362,0.000044307577,0.00038447985,0.00030918358,0.00042624428,0.005399398,0.00013994571,0.00009369105,0.006196004],"study_design_scores_gemma":[0.0000035220476,0.00003993529,0.9969862,0.000011950484,0.000014349897,0.00045016367,0.00042374674,0.00025434856,0.001072945,0.000051366318,0.00068963773,0.0000018282879],"about_ca_topic_score_codex":0.003145562,"about_ca_topic_score_gemma":0.0044464944,"teacher_disagreement_score":0.003145562,"about_ca_system_score_codex":0.00021782421,"about_ca_system_score_gemma":0.00012922294,"threshold_uncertainty_score":0.006254554},"labels":[],"label_agreement":null},{"id":"W4304889465","doi":"10.3847/1538-4357/ac8b7d","title":"A Multiwavelength View of IC 860: What Is in Action inside Quenching Galaxies <sup>*</sup>","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"U.S. Department of Energy; U.S. Naval Observatory; Max-Planck-Institut für Astronomie; University of Portsmouth; University of California, Los Angeles; Max-Planck-Gesellschaft; Chinese Academy of Sciences; Space Telescope Science Institute; New Mexico State University; Universität Basel; University of Pittsburgh; Los Alamos National Laboratory; Alfred P. Sloan Foundation; University of Washington; Princeton University; Johns Hopkins University; Ohio State University; Japan Aerospace Exploration Agency; California Institute of Technology; Jet Propulsion Laboratory; Fermilab; Case Western Reserve University; National Science Foundation; Drexel University; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Star formation; Galaxy; Outflow; Quenching (fluorescence); Stellar mass; Astronomy; Fluorescence","score_opus":0.012873087988355056,"score_gpt":0.23471368434744133,"score_spread":0.22184059635908626,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304889465","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924315,0.00045497043,0.00045932314,0.00012942312,0.000007171652,0.0000034801935,0.00031809811,0.00006950524,0.006126379],"genre_scores_gemma":[0.99775296,0.00013289454,0.0008835154,0.000076397555,0.00002828816,0.0000014925753,0.00022464729,0.000018649233,0.00088115345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999671,0.0000025570894,0.0000013011129,0.000007972442,0.000007083375,0.000014015871],"domain_scores_gemma":[0.99981254,0.00002053207,0.00006377075,0.000016411546,0.000019917472,0.00006686725],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009787114,0.000119874654,0.000111453104,0.00079168845,0.0002745188,0.00043867677,0.00019082736,0.00022026019,0.0021930388],"category_scores_gemma":[0.0001468313,0.000119970944,0.0001586748,0.0004893496,0.00019590804,0.00034464878,0.0003298331,0.00025022207,0.00046606106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052532123,0.00012981116,0.4945399,0.00017639204,0.000087657725,0.0026672012,0.0024218971,0.0014448272,0.4553629,0.0015545521,0.0032282616,0.037861362],"study_design_scores_gemma":[0.000001882723,0.000038015245,0.9944417,0.000006785807,0.000016123817,0.00058791385,0.0002919291,0.0004274897,0.002444289,0.00015295968,0.0015869193,0.000003969739],"about_ca_topic_score_codex":0.0021193207,"about_ca_topic_score_gemma":0.004344042,"teacher_disagreement_score":0.0021930388,"about_ca_system_score_codex":0.00025208,"about_ca_system_score_gemma":0.000058175036,"threshold_uncertainty_score":0.0073364377},"labels":[],"label_agreement":null},{"id":"W4304889494","doi":"10.3847/1538-4357/ac8b05","title":"Active Learning for Computationally Efficient Distribution of Binary Evolution Simulations","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Fonds Wetenschappelijk Onderzoek; Canadian Institute for Advanced Research; Northwestern University; Gordon and Betty Moore Foundation; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation","keywords":"Binary number; Interpolation (computer graphics); Scalability; Grid; Population; Set (abstract data type); Range (aeronautics); Physics; Computer science; Algorithm; Artificial intelligence; Database; Mathematics","score_opus":0.010026461899811037,"score_gpt":0.23980310522649595,"score_spread":0.2297766433266849,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4304889494","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.08199043,0.00018779727,0.9098744,0.00056705053,0.00008025125,0.00013947325,0.00022534149,0.002635832,0.0042994027],"genre_scores_gemma":[0.64316636,0.00008325238,0.35207084,0.00025470878,0.00006336105,0.00041758534,0.000583288,0.00047639533,0.0028841873],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9994247,0.00023003352,0.000031355692,0.000089141,0.00015696052,0.00006789352],"domain_scores_gemma":[0.99443203,0.0040223002,0.00027122328,0.00041919123,0.0006260314,0.0002292164],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022896,0.00074803474,0.00094555324,0.0006625926,0.00066784513,0.0011377345,0.0030547408,0.00133149,0.004151792],"category_scores_gemma":[0.009768846,0.00072532153,0.00070151995,0.0005657503,0.0011935784,0.0014239115,0.001674189,0.002389719,0.0007931379],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008552905,0.000046676345,0.00077094714,0.00003204578,0.000015296784,0.00003174156,0.000031441577,0.97841245,0.0006472022,0.005799002,0.0005768775,0.01355078],"study_design_scores_gemma":[0.0000045632023,0.000002272852,0.000012758796,0.0000011044508,3.644771e-7,7.666609e-7,0.000001139499,0.9989567,0.00013032464,0.0008346279,0.000054676213,6.333213e-7],"about_ca_topic_score_codex":0.006203864,"about_ca_topic_score_gemma":0.006204261,"teacher_disagreement_score":0.006203864,"about_ca_system_score_codex":0.001668775,"about_ca_system_score_gemma":0.0013458316,"threshold_uncertainty_score":0.013889134},"labels":[],"label_agreement":null},{"id":"W4306176134","doi":"10.3847/1538-4357/acb64c","title":"BICEP/Keck. XVI. Characterizing Dust Polarization through Correlations with Neutral Hydrogen","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Cosmic microwave background; Polarization (electrochemistry); Astronomy; Planck; Gravitational wave; Interstellar medium; Anisotropy; Galaxy","score_opus":0.01533226963566516,"score_gpt":0.23949158702783624,"score_spread":0.22415931739217107,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306176134","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.44674313,0.0010050768,0.00689103,0.00045500646,0.000111335445,0.00019940568,0.4787529,0.008353507,0.057488613],"genre_scores_gemma":[0.5742829,0.00036017282,0.01993516,0.0002377094,0.00009459026,0.00034858147,0.38776007,0.0023440437,0.014636808],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976915,0.00002601123,0.000012066929,0.000058413523,0.00007481585,0.00005959273],"domain_scores_gemma":[0.9990589,0.00015104828,0.00019212288,0.00031855504,0.00014508214,0.00013429683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005801124,0.0006066146,0.00028614717,0.00231107,0.00038484528,0.001058636,0.00052424497,0.00026802093,0.022972522],"category_scores_gemma":[0.00093706464,0.0003273436,0.00027913027,0.002227635,0.0001603497,0.0005629084,0.0012184915,0.0003162481,0.010484337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002462969,0.000220827,0.40665555,0.0008869277,0.00077989703,0.00078613,0.00047556512,0.007447559,0.042275403,0.003030859,0.33319753,0.2017807],"study_design_scores_gemma":[0.000077126075,0.0000831267,0.8584514,0.000067687826,0.000070470574,0.0005542723,0.00012276697,0.007089654,0.015871525,0.0012442641,0.11631464,0.00005295265],"about_ca_topic_score_codex":0.004038465,"about_ca_topic_score_gemma":0.0049088118,"teacher_disagreement_score":0.022972522,"about_ca_system_score_codex":0.00023126267,"about_ca_system_score_gemma":0.000181649,"threshold_uncertainty_score":0.07685077},"labels":[],"label_agreement":null},{"id":"W4306246298","doi":"10.3847/1538-4357/ac983d","title":"The Radius of PSR J0740+6620 from NICER with NICER Background Estimates","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":111,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Los Alamos National Laboratory; National Nuclear Security Administration; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; U.S. Department of Energy","keywords":"Physics; Astrophysics; Millisecond pulsar; Pulsar; RADIUS; Neutron star","score_opus":0.012447380638694069,"score_gpt":0.29875189373404154,"score_spread":0.2863045130953475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306246298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98117673,0.0007425563,0.009673337,0.00013318253,0.000020070485,0.000011137516,0.0020311058,0.00079921726,0.005412604],"genre_scores_gemma":[0.98903567,0.0001361768,0.004403505,0.00007206133,0.000027232918,0.000012513059,0.0056182207,0.0002888813,0.00040574474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99901164,0.00016963655,0.000060817907,0.00031431767,0.00031777294,0.00012576203],"domain_scores_gemma":[0.9973326,0.00047525013,0.00091927295,0.000698835,0.00038114144,0.00019287402],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016274429,0.00043722708,0.0005414191,0.0018480775,0.00033842775,0.0011896624,0.00082609983,0.00042736676,0.0014316106],"category_scores_gemma":[0.0038968245,0.00034527114,0.000871369,0.0010957787,0.0003540122,0.0004829261,0.0016864175,0.00040501778,0.0012383868],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052638206,0.00003442125,0.8808414,0.00014946565,0.00041166975,0.00053888053,0.00035512444,0.021300951,0.052712314,0.0023537884,0.0031660849,0.03760956],"study_design_scores_gemma":[0.000021986956,0.00006405501,0.94801366,0.00003039503,0.00011408081,0.00068870105,0.000098584,0.037361175,0.005841361,0.0007968937,0.006923127,0.000046040448],"about_ca_topic_score_codex":0.0040489696,"about_ca_topic_score_gemma":0.004200602,"teacher_disagreement_score":0.0040489696,"about_ca_system_score_codex":0.0005333585,"about_ca_system_score_gemma":0.00029388067,"threshold_uncertainty_score":0.008606851},"labels":[],"label_agreement":null},{"id":"W4306699762","doi":"10.3847/1538-4357/ac91cb","title":"The Hubble Space Telescope Survey of M31 Satellite Galaxies. I. RR Lyrae–based Distances and Refined 3D Geometric Structure","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":68,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; University of California Berkeley","keywords":"Physics; RR Lyrae variable; Astrophysics; Astronomy; Local Group; Galaxy; Red-giant branch; Right ascension; Satellite galaxy; Globular cluster; Metallicity; Galaxy formation and evolution; Milky Way; Declination","score_opus":0.008031472672954192,"score_gpt":0.20942912082997228,"score_spread":0.20139764815701808,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306699762","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9892161,0.0004798694,0.0015069759,0.000115597904,0.0000045088327,0.000020986876,0.0038600534,0.00008219601,0.004713654],"genre_scores_gemma":[0.99378645,0.00022861737,0.0028493355,0.000028377359,0.000012789763,0.000009111179,0.0025997686,0.000014799656,0.0004708089],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998246,0.00003545336,0.00001128194,0.000045137316,0.00005881247,0.000024812804],"domain_scores_gemma":[0.99919266,0.000056771456,0.00032813632,0.00018411485,0.00012806462,0.00011031862],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005545624,0.00022299052,0.0001371701,0.002408097,0.00020838936,0.0005630004,0.00021047205,0.00014926713,0.00071602355],"category_scores_gemma":[0.0010237284,0.000118824,0.00014511385,0.0014289988,0.00024562274,0.00043448468,0.0004918885,0.00022480442,0.00078168185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000031874242,0.000010916886,0.97369677,0.000014836815,0.000024114705,0.000045412304,0.00022179827,0.0010052485,0.0035637373,0.00055340974,0.0012006356,0.019631216],"study_design_scores_gemma":[0.0000011512946,0.000007083473,0.9976776,0.0000045277884,0.0000020551936,0.000027172533,0.000051931627,0.00069934776,0.00021408389,0.00011491731,0.0011969983,0.0000030487843],"about_ca_topic_score_codex":0.023759067,"about_ca_topic_score_gemma":0.060606074,"teacher_disagreement_score":0.023759067,"about_ca_system_score_codex":0.00064985274,"about_ca_system_score_gemma":0.00027783433,"threshold_uncertainty_score":0.04724157},"labels":[],"label_agreement":null},{"id":"W4306699928","doi":"10.3847/1538-4357/ac8747","title":"MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z ≳ 3*","year":2022,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Velocity dispersion; Astronomy","score_opus":0.008802099645191745,"score_gpt":0.21100322005974798,"score_spread":0.20220112041455623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306699928","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58479655,0.0015421924,0.034273103,0.0016893791,0.00070531806,0.000108465254,0.25815764,0.052166387,0.066561036],"genre_scores_gemma":[0.77882886,0.00027375008,0.017559335,0.00040235257,0.000440781,0.00009148533,0.1781373,0.0054965243,0.01876963],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9998136,0.000025531994,0.00000951014,0.00005408877,0.00005690879,0.000040359377],"domain_scores_gemma":[0.99899524,0.00022701996,0.00016111872,0.0002300608,0.0001710412,0.00021551024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006754211,0.00030118407,0.000258221,0.0014299238,0.00032636174,0.0009094389,0.00051015726,0.00027012764,0.013406649],"category_scores_gemma":[0.0015130537,0.00012620677,0.00029748585,0.0012946547,0.00013480637,0.000575743,0.00063943944,0.0003330955,0.00821918],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014558828,0.0001617369,0.3705057,0.0003925633,0.00014380102,0.00044022777,0.0010747883,0.0065033073,0.023130748,0.011761644,0.41145763,0.17297196],"study_design_scores_gemma":[0.00020317518,0.00014837463,0.5637777,0.00006378142,0.0000602526,0.00040912224,0.0002939861,0.021533087,0.02156201,0.0070589846,0.3847904,0.00009910697],"about_ca_topic_score_codex":0.0032196182,"about_ca_topic_score_gemma":0.0048810844,"teacher_disagreement_score":0.013406649,"about_ca_system_score_codex":0.00034799826,"about_ca_system_score_gemma":0.00016244015,"threshold_uncertainty_score":0.044849753},"labels":[],"label_agreement":null},{"id":"W4306787189","doi":"10.3847/1538-4357/ac9138","title":"Fast Neutrino Cooling in the Accreting Neutron Star MXB 1659-29","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Schlumberger Foundation","keywords":"Physics; Neutron star; Neutrino; Astrophysics; Luminosity; Nuclear physics; Superfluidity; Neutron","score_opus":0.014594936294626118,"score_gpt":0.30314754414480405,"score_spread":0.28855260785017794,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306787189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985885,0.00006360757,0.0007150718,0.000041612904,0.0000041771927,0.000003740307,0.00006844575,0.00002619397,0.0004886072],"genre_scores_gemma":[0.99953485,0.000019366405,0.00022192782,0.000011342603,0.0000023260607,0.0000024417577,0.00008129709,0.000009525568,0.00011689778],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999298,0.000016373791,0.000005790336,0.000018975174,0.000014504868,0.000014489715],"domain_scores_gemma":[0.9998042,0.000049516733,0.000060214785,0.000021243635,0.000018611965,0.000046338235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050118286,0.00047230555,0.0005249267,0.00025338915,0.0004635612,0.00063766935,0.00047634376,0.00039249763,0.00060362363],"category_scores_gemma":[0.0005813875,0.0002639757,0.00052618457,0.00014572327,0.00038346648,0.00035633566,0.000581216,0.00038695638,0.00009387999],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013131113,0.000334447,0.3137389,0.00019858111,0.00043289308,0.0023039384,0.00042539838,0.4611489,0.20369329,0.0077165426,0.00055420666,0.008139841],"study_design_scores_gemma":[0.00021905068,0.0005490619,0.16813305,0.000028682407,0.0000859491,0.00036407876,0.00014635445,0.811826,0.014982505,0.0026180705,0.000988288,0.000058871006],"about_ca_topic_score_codex":0.0062408927,"about_ca_topic_score_gemma":0.0041142157,"teacher_disagreement_score":0.0062408927,"about_ca_system_score_codex":0.0007808495,"about_ca_system_score_gemma":0.00027913376,"threshold_uncertainty_score":0.012409151},"labels":[],"label_agreement":null},{"id":"W4306787226","doi":"10.3847/1538-4357/ac90be","title":"A 4 Gyr M-dwarf Gyrochrone from CFHT/MegaPrime Monitoring of the Open Cluster M67","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Science Foundation","keywords":"Physics; Open cluster; Astrophysics; Photometry (optics); Metallicity; Pleiades; Blue straggler; Astronomy; Rotation period; Stars; Star cluster; Starspot","score_opus":0.01623258945083472,"score_gpt":0.24351331728144682,"score_spread":0.2272807278306121,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306787226","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99946696,0.00002072924,0.00006616645,0.000006376314,0.0000014357157,0.000001653801,0.0002020974,0.000007813406,0.00022668399],"genre_scores_gemma":[0.99907434,0.000013358147,0.00021639085,0.000005052707,0.0000032527976,0.000001789678,0.000567806,0.00000358143,0.00011442835],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987924,0.000010708333,0.0000048216416,0.000035414305,0.000033553166,0.000036378846],"domain_scores_gemma":[0.99957556,0.000039929604,0.00010098988,0.00006260577,0.0000748269,0.0001459715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021680127,0.00018085142,0.00017917909,0.001153547,0.00036737637,0.00023442955,0.00020980465,0.00017052479,0.0006872113],"category_scores_gemma":[0.00042414767,0.000086535205,0.00013966976,0.00040594063,0.00018420546,0.00012762938,0.00042845306,0.00014516867,0.00023783701],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021975173,0.000030523053,0.97046494,0.000018316216,0.000024352139,0.00039238957,0.00045351512,0.00027157567,0.015160824,0.000089279856,0.0004519457,0.012422435],"study_design_scores_gemma":[0.0000021164967,0.000037589005,0.9977176,0.0000030088515,0.000007406332,0.0001539335,0.00008431177,0.00043904112,0.0010991414,0.000013486241,0.00043984514,0.0000025482198],"about_ca_topic_score_codex":0.010615126,"about_ca_topic_score_gemma":0.025150316,"teacher_disagreement_score":0.010615126,"about_ca_system_score_codex":0.0004278506,"about_ca_system_score_gemma":0.00012712447,"threshold_uncertainty_score":0.02110672},"labels":[],"label_agreement":null},{"id":"W4306814920","doi":"10.3847/1538-4357/acc85c","title":"BICEP/Keck. XVII. Line-of-sight Distortion Analysis: Estimates of Gravitational Lensing, Anisotropic Cosmic Birefringence, Patchy Reionization, and Systematic Errors","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Jet Propulsion Laboratory; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Cosmic microwave background; Reionization; Astrophysics; Hubble's law; Gravitational wave; Gravitational lens; Weak gravitational lensing; Axion; Amplitude; Planck; Cosmology; Dark energy; Anisotropy; Redshift; Dark matter; Galaxy; Optics","score_opus":0.009869940569691498,"score_gpt":0.2551269472330359,"score_spread":0.2452570066633444,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306814920","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.03425048,0.0008651585,0.03009022,0.0005017583,0.00019425093,0.00027969413,0.81040514,0.05755463,0.06585864],"genre_scores_gemma":[0.07656499,0.0005156136,0.07686629,0.00030738435,0.00009952669,0.0011950717,0.78409606,0.033131022,0.027223978],"study_design_codex":"not_applicable","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99903345,0.00017287445,0.00008846133,0.00019928323,0.0003748301,0.00013110197],"domain_scores_gemma":[0.99545336,0.000977988,0.00059390714,0.0013686471,0.0013939731,0.000212081],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022445794,0.0015978958,0.00070190785,0.0049130325,0.00056952995,0.0015176083,0.0016628023,0.0004582336,0.06329755],"category_scores_gemma":[0.0061663436,0.001199241,0.0007927737,0.0073694424,0.00026122917,0.0014456091,0.001828741,0.0008203498,0.052542977],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090319087,0.000058116486,0.015755737,0.0006449516,0.00022856634,0.00021157446,0.00015693053,0.0038398772,0.0029797412,0.003853107,0.8644415,0.106926695],"study_design_scores_gemma":[0.0005615586,0.00015128254,0.24619192,0.00041789594,0.00019551723,0.0009263764,0.00020297681,0.023818959,0.030444728,0.010114351,0.68673545,0.00023910719],"about_ca_topic_score_codex":0.018781051,"about_ca_topic_score_gemma":0.01254398,"teacher_disagreement_score":0.06329755,"about_ca_system_score_codex":0.0007222532,"about_ca_system_score_gemma":0.0006787641,"threshold_uncertainty_score":0.21175134},"labels":[],"label_agreement":null},{"id":"W4306850861","doi":"10.3847/1538-4357/ac8b7a","title":"The Pantheon+ Analysis: The Full Data Set and Light-curve Release","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":835,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; University of Edinburgh; Max-Planck-Institut für Astronomie; Gordon and Betty Moore Foundation; Queen's University Belfast; Los Alamos National Laboratory; Alfred P. Sloan Foundation; Johns Hopkins University; David and Lucile Packard Foundation; U.S. Department of Energy; Smithsonian Institution; John Templeton Foundation; Space Telescope Science Institute; Durham University; National Aeronautics and Space Administration; Queen's University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; National Central University; Nuclear Safety and Security Commission; Heising-Simons Foundation; Eötvös Loránd Tudományegyetem; National Science Foundation","keywords":"Physics; Dark energy; Light curve; Redshift; Supernova; Astrophysics; Hubble's law; Galaxy; Equation of state; Cosmology; Astronomy","score_opus":0.017372985842030276,"score_gpt":0.246972191157512,"score_spread":0.22959920531548172,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4306850861","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.014475032,0.00009012178,0.003054138,0.00019965087,0.00006430096,0.0001980082,0.9624242,0.011138712,0.008355826],"genre_scores_gemma":[0.022336893,0.00008176687,0.008095997,0.0001273282,0.000053026175,0.00061955437,0.96030843,0.0036790196,0.0046980586],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9986745,0.00016823059,0.0001130104,0.0003334529,0.00048567963,0.00022513673],"domain_scores_gemma":[0.99485,0.0007816914,0.0006939682,0.0020842717,0.0012583055,0.00033174912],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019027584,0.001553085,0.0012084225,0.0050503355,0.00062324305,0.001557697,0.0016950187,0.000516722,0.072955176],"category_scores_gemma":[0.005226984,0.0009169657,0.0009016989,0.0062476443,0.00040248234,0.001679124,0.0023349337,0.0010013512,0.04936933],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011876426,0.00013284346,0.040684916,0.0005024244,0.00019613004,0.00018211622,0.00011500886,0.0011924392,0.0026514526,0.0017919729,0.9140523,0.037310757],"study_design_scores_gemma":[0.000632072,0.00017015783,0.16011065,0.00017458666,0.00015482632,0.000408143,0.00012859704,0.00490329,0.005938749,0.0029790825,0.824219,0.00018089953],"about_ca_topic_score_codex":0.013304081,"about_ca_topic_score_gemma":0.015082557,"teacher_disagreement_score":0.072955176,"about_ca_system_score_codex":0.00076657214,"about_ca_system_score_gemma":0.0019153028,"threshold_uncertainty_score":0.24405938},"labels":[],"label_agreement":null},{"id":"W4307045304","doi":"10.3847/1538-4357/ac6fdf","title":"X-Rays in Cepheids: Identifying Low-mass Companions of Intermediate-mass Stars*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"European Commission; Nuclear Safety and Security Commission; European Space Agency; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Cepheid variable; Physics; Astrophysics; Low Mass; Stars; Astronomy; Flux (metallurgy)","score_opus":0.014454009439353271,"score_gpt":0.23980521645441286,"score_spread":0.2253512070150596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307045304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99968505,0.00007060395,0.000045287004,0.0000047420494,0.0000010721749,0.0000028193463,0.000033633074,0.0000011940061,0.00015560145],"genre_scores_gemma":[0.9997178,0.000022877988,0.00009152243,0.000005654864,0.0000021717774,0.0000016094014,0.000080088,5.820594e-7,0.00007767163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982786,0.000023952467,0.000014563376,0.000053867978,0.000035709432,0.00004400452],"domain_scores_gemma":[0.9991499,0.00017289758,0.00026892556,0.00005511381,0.00012713083,0.0002260496],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030068288,0.0002008823,0.0002283259,0.0011731728,0.00053335086,0.00056176353,0.00023501547,0.0002728072,0.0012285584],"category_scores_gemma":[0.0011457813,0.000102877224,0.00008250818,0.0005533893,0.0003099999,0.00026223256,0.00049048226,0.00018205754,0.00024021558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000088772904,0.000028721619,0.9948147,0.0000069222406,0.0000041103954,0.00018304541,0.00015835748,0.000016819498,0.0021979436,0.000027042182,0.000035175366,0.00243835],"study_design_scores_gemma":[0.0000026765047,0.00007024504,0.998874,0.0000023889884,0.000003462373,0.00034355515,0.00013482373,0.00009259443,0.00028211,0.000018138111,0.00017483598,0.0000011450647],"about_ca_topic_score_codex":0.003403971,"about_ca_topic_score_gemma":0.0047897315,"teacher_disagreement_score":0.003403971,"about_ca_system_score_codex":0.00018771381,"about_ca_system_score_gemma":0.000121648445,"threshold_uncertainty_score":0.006768286},"labels":[],"label_agreement":null},{"id":"W4307689769","doi":"10.3847/1538-4357/ac958a","title":"One-off and Repeating Fast Radio Bursts: A Statistical Analysis","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"China National Funds for Distinguished Young Scientists; National Natural Science Foundation of China","keywords":"Physics; Statistical analysis; Astrophysics; Statistic; Statistics; Mathematics","score_opus":0.011373926982417785,"score_gpt":0.30373820468675594,"score_spread":0.29236427770433815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307689769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9919233,0.00018442124,0.0048293998,0.000060089893,0.00002387814,0.000083897925,0.001374908,0.00008256209,0.0014375327],"genre_scores_gemma":[0.997248,0.00002769463,0.0010236017,0.000017171096,0.000023539842,0.00005684965,0.001139617,0.000029847128,0.0004336369],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9947351,0.0011148979,0.00043247573,0.0012218069,0.0019388299,0.0005569025],"domain_scores_gemma":[0.949756,0.03685023,0.0056661996,0.0035365196,0.0024038542,0.0017871833],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.006801547,0.00032141083,0.00078049913,0.0042648334,0.0006660815,0.0013764153,0.0011682705,0.00055412884,0.0046390067],"category_scores_gemma":[0.02373358,0.00015530945,0.0010020884,0.0038993834,0.0016939,0.00097648054,0.0011501022,0.0009917902,0.00041926824],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005450691,0.00011798045,0.98034966,0.000039028644,0.0005120909,0.00020586755,0.00038233178,0.0011642971,0.001781084,0.000839574,0.0007144669,0.01334849],"study_design_scores_gemma":[0.0000107495025,0.00026968238,0.9875535,0.000009330312,0.000112376714,0.00018627499,0.000562634,0.009185581,0.00050033664,0.0006495977,0.0009352995,0.00002464698],"about_ca_topic_score_codex":0.0062895026,"about_ca_topic_score_gemma":0.0033922312,"teacher_disagreement_score":0.006801547,"about_ca_system_score_codex":0.0006859769,"about_ca_system_score_gemma":0.0007637926,"threshold_uncertainty_score":0.03597045},"labels":[],"label_agreement":null},{"id":"W4307689925","doi":"10.3847/1538-4357/ac9404","title":"Linear and Nonlinear Kelvin–Helmholtz Instability and Magnetohydrodynamic Wave Emission in Sheared Astrophysical Plasma Flows","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Ionosphere and magnetosphere dynamics","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency; Natural Sciences and Engineering Research Council of Canada; National Nuclear Security Administration; Office of Science; University of Rochester; U.S. Department of Energy","keywords":"Physics; Magnetohydrodynamics; Magnetohydrodynamic drive; Instability; Shear flow; Plasma; Mechanics; Astrophysics; Alfvén wave; Classical mechanics; Computational physics","score_opus":0.005833106255340016,"score_gpt":0.20778181914387026,"score_spread":0.20194871288853025,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307689925","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99804085,0.00018902367,0.00076515356,0.0000170837,0.000003118388,0.0000040102304,0.000041107032,0.000014349687,0.00092532125],"genre_scores_gemma":[0.99960214,0.000028871787,0.00020011791,0.0000018724116,0.0000034573777,0.0000015149476,0.00003149728,0.000002290598,0.00012824828],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995315,0.000006083648,0.0000024732838,0.000011096112,0.000011781241,0.000015363978],"domain_scores_gemma":[0.99973387,0.00007441728,0.00009971827,0.000012957116,0.00003165719,0.000047272963],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016878516,0.00020341651,0.00015026134,0.00064417964,0.00023734363,0.0005033636,0.00016504325,0.00018009085,0.000768197],"category_scores_gemma":[0.00047993477,0.00012924883,0.0001450386,0.00032526182,0.0005154381,0.00034913907,0.0004089294,0.00022202672,0.00008901945],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020758014,0.00017024677,0.4097812,0.00021639629,0.0001302927,0.0014233614,0.0010278217,0.026635338,0.52546614,0.0067358282,0.000493201,0.025844458],"study_design_scores_gemma":[0.000079907666,0.00019436082,0.82757753,0.000024425375,0.000026790516,0.00042764013,0.000452374,0.09940014,0.068199016,0.0028207968,0.00074992824,0.000047070993],"about_ca_topic_score_codex":0.0014353702,"about_ca_topic_score_gemma":0.0005802894,"teacher_disagreement_score":0.0014353702,"about_ca_system_score_codex":0.00024880897,"about_ca_system_score_gemma":0.00009804797,"threshold_uncertainty_score":0.0028541088},"labels":[],"label_agreement":null},{"id":"W4307702218","doi":"10.3847/1538-4357/ac8790","title":"Connecting MeerKAT Radio Continuum Properties to GAMA Optical Emission-line and WISE Mid-infrared Activity","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Infrared; Galaxy; Photometry (optics); Star formation; Luminosity; Luminous infrared galaxy; Active galactic nucleus; Astronomy; Wavelength; Emission spectrum; Stars; Spectral line; Optics","score_opus":0.012435379841661511,"score_gpt":0.21859631581460834,"score_spread":0.20616093597294682,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307702218","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99766064,0.000049626295,0.000634852,0.000011950223,0.0000017342236,0.000006585199,0.0006236306,0.000050880677,0.00095998705],"genre_scores_gemma":[0.99839956,0.00001686096,0.0005785251,0.000007798872,0.0000031827649,0.000004905392,0.0008221182,0.000009250655,0.00015780897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997003,0.000044763878,0.000023115608,0.000102086604,0.00006938668,0.000060336308],"domain_scores_gemma":[0.99851793,0.0002458398,0.0006193009,0.00016453136,0.00021547465,0.00023693623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006816634,0.00028567505,0.00023391671,0.0028227551,0.00018023652,0.0007049896,0.00027474947,0.0002379198,0.0018860481],"category_scores_gemma":[0.0017398719,0.00019630109,0.00024667036,0.00089921115,0.00025761657,0.00049560587,0.0007481752,0.00030298872,0.0008954104],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009386253,0.000025925458,0.98801094,0.000015064537,0.00004755261,0.000027951859,0.00006807961,0.00045571147,0.0054017026,0.00006397079,0.00014112302,0.0056482274],"study_design_scores_gemma":[0.0000022790389,0.000015160902,0.998038,0.0000022837164,0.000010808907,0.00003030106,0.000042789947,0.0012189937,0.0004614209,0.000032781325,0.00014290356,0.0000023673244],"about_ca_topic_score_codex":0.0027204482,"about_ca_topic_score_gemma":0.0034460337,"teacher_disagreement_score":0.0028227551,"about_ca_system_score_codex":0.00020694116,"about_ca_system_score_gemma":0.000063723615,"threshold_uncertainty_score":0.0063094497},"labels":[],"label_agreement":null},{"id":"W4307800202","doi":"10.3847/1538-4357/ac94c2","title":"Improved Measurements of Galaxy Star Formation Stochasticity from the Intrinsic Scatter of Burst Indicators","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"U.S. Department of Energy","keywords":"Physics; Burstiness; Astrophysics; Star formation; Galaxy; Star (game theory); Stars","score_opus":0.012108452108023655,"score_gpt":0.20887758687202646,"score_spread":0.1967691347640028,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307800202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.80554724,0.00045404222,0.18383253,0.00015470479,0.000040437633,0.00002541076,0.0041940697,0.0011193032,0.0046322783],"genre_scores_gemma":[0.9792118,0.000120033204,0.016632719,0.00004034886,0.000053844135,0.000018356146,0.0030028324,0.00016882317,0.00075123564],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987758,0.0003099179,0.000085120766,0.00042471668,0.00030849478,0.0000959938],"domain_scores_gemma":[0.9920974,0.0031761313,0.0018587592,0.0016846579,0.0008017374,0.0003812648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002528891,0.0005427677,0.0005052451,0.0020514366,0.00022208366,0.0016430528,0.00062142656,0.0003615706,0.0012609],"category_scores_gemma":[0.009245885,0.0004966531,0.0004659058,0.0013416806,0.00036204676,0.0014655936,0.0012313478,0.0008749748,0.0005342168],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042580476,0.00007348971,0.82952887,0.00010517955,0.0005300418,0.000069710106,0.00029655118,0.04579466,0.047386713,0.0049621766,0.0017824739,0.06904434],"study_design_scores_gemma":[0.000023486991,0.00008686107,0.6860709,0.000031997002,0.00011510932,0.00020742156,0.00006321477,0.2791101,0.024787132,0.0063218935,0.0030638042,0.00011808858],"about_ca_topic_score_codex":0.004900525,"about_ca_topic_score_gemma":0.005674776,"teacher_disagreement_score":0.004900525,"about_ca_system_score_codex":0.00061007956,"about_ca_system_score_gemma":0.00029232138,"threshold_uncertainty_score":0.013374209},"labels":[],"label_agreement":null},{"id":"W4307983220","doi":"10.3847/1538-4357/ac9235","title":"Millimeter Dust Emission and Planetary Dynamics in the HD 106906 System","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Astronomical Observatory of Japan; National Institutes of Natural Sciences; Connecticut Space Grant College Consortium; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Research Corporation for Science Advancement; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Debris disk; Planetesimal; Planet; Astrophysics; Astronomy; Orbital eccentricity; Planetary system; Submillimeter Array; Millimeter; Protoplanetary disk; Circumstellar dust; Circumbinary planet; Circular orbit; Thick disk; Eccentricity (behavior); Stars; Star formation; Galaxy; Halo","score_opus":0.007633907448996606,"score_gpt":0.20630224565946767,"score_spread":0.19866833821047106,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307983220","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990075,0.00005340726,0.0000670221,0.000024239742,0.0000024456558,0.0000023086652,0.0001982465,0.000018546127,0.00062625244],"genre_scores_gemma":[0.999553,0.0000142911595,0.00009641884,0.000014917763,0.000003493666,0.0000011380262,0.00023803863,0.000002267688,0.00007638619],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999496,0.0000048876504,0.0000033452081,0.000016840802,0.000012049303,0.000013303953],"domain_scores_gemma":[0.9998944,0.00001751925,0.000040934727,0.000009314098,0.000007293915,0.000030571045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010178579,0.00023624818,0.00020020637,0.00044193087,0.0003059854,0.00040495023,0.00019494505,0.0002995158,0.0009304734],"category_scores_gemma":[0.00018173788,0.00013040123,0.00016338944,0.00030993842,0.00015733887,0.00015877832,0.00033624828,0.00024347949,0.00022808656],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002986167,0.00022024117,0.90179664,0.00003658071,0.0000775955,0.00056000944,0.00032664096,0.0017599269,0.08683371,0.0004043522,0.0007479846,0.006937719],"study_design_scores_gemma":[0.000015144597,0.000040504736,0.99590224,0.000002484244,0.000011134099,0.00013585157,0.000059723898,0.0021766415,0.0012234417,0.00005328529,0.0003753011,0.0000042342],"about_ca_topic_score_codex":0.005393779,"about_ca_topic_score_gemma":0.0054928157,"teacher_disagreement_score":0.005393779,"about_ca_system_score_codex":0.00031489154,"about_ca_system_score_gemma":0.000055925546,"threshold_uncertainty_score":0.010724783},"labels":[],"label_agreement":null},{"id":"W4307984966","doi":"10.3847/1538-4357/ac9476","title":"Improved Models of R Coronae Borealis Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"U.S. Department of Energy","keywords":"Nucleosynthesis; Physics; Astrophysics; Stars; Stellar nucleosynthesis; r-process; Neutron star; Envelope (radar); Nuclear fusion; Corona (planetary geology); Nuclear physics; Astrobiology","score_opus":0.013534667734797437,"score_gpt":0.2196320764707434,"score_spread":0.20609740873594595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4307984966","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8685599,0.0003356764,0.099320576,0.00043174395,0.00006724305,0.00014117072,0.0010028712,0.0006250857,0.029515827],"genre_scores_gemma":[0.9820472,0.0000983224,0.013727929,0.000056587407,0.00002603558,0.00011504298,0.00028695556,0.00007356553,0.0035683666],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998578,0.0000530327,0.0000076303495,0.000028070393,0.000029642053,0.00002375656],"domain_scores_gemma":[0.99966264,0.0001221159,0.00005898582,0.000035168607,0.00006996828,0.00005113992],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038770062,0.00060701516,0.0006246,0.00043859796,0.00061471795,0.00071333325,0.0019117603,0.0012524727,0.0022755577],"category_scores_gemma":[0.0009896561,0.00041099562,0.0009983729,0.0003313405,0.00055110094,0.0005858542,0.0008172336,0.0004952102,0.00036466864],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000248481,0.000020889187,0.0010825212,0.000007928458,0.0000116046385,0.00004950715,0.000020397894,0.99594903,0.0009426573,0.001361056,0.00006821283,0.00046133748],"study_design_scores_gemma":[0.000024524936,0.000014784795,0.00030892296,0.0000014610073,0.000004196618,0.0000120580835,0.0000069759017,0.9988961,0.0001265183,0.00036598372,0.00023378246,0.0000046040445],"about_ca_topic_score_codex":0.037020937,"about_ca_topic_score_gemma":0.014108234,"teacher_disagreement_score":0.037020937,"about_ca_system_score_codex":0.001246648,"about_ca_system_score_gemma":0.0007676712,"threshold_uncertainty_score":0.07361084},"labels":[],"label_agreement":null},{"id":"W4308020633","doi":"10.3847/1538-4357/acd3f2","title":"A Search for Relativistic Ejecta in a Sample of ZTF Broad-lined Type Ic Supernovae","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Deutsches Elektronen-Synchrotron; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Stockholms Universitet; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Aarhus Universitet; Turun Yliopisto; Nuclear Safety and Security Commission; Knut och Alice Wallenbergs Stiftelse; Háskóli Íslands; Universitetet i Oslo; Smithsonian Institution; Vetenskapsrådet; Max-Planck-Gesellschaft; Queen's University; Durham University; Trinity College Dublin; Space Telescope Science Institute; Los Alamos National Laboratory; Johns Hopkins University; Eötvös Loránd Tudományegyetem; California Institute of Technology; Gordon and Betty Moore Foundation; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; National Science Foundation","keywords":"Ejecta; Physics; Supernova; Astrophysics; Gamma-ray burst; Luminosity; Astrophysical jet; Astronomy; Light curve; Active galactic nucleus; Galaxy","score_opus":0.03004206853582428,"score_gpt":0.28558174567291433,"score_spread":0.25553967713709,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308020633","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943644,0.000043093987,0.00010878118,0.0000062345257,7.012618e-7,0.000008450692,0.0002576618,0.0000059161775,0.00013258461],"genre_scores_gemma":[0.99814856,0.000050998762,0.0003145098,0.000014405825,0.0000045948505,0.000010282721,0.001261048,0.000005270404,0.00019034406],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995989,0.00003795815,0.00002937159,0.0001405279,0.00007261999,0.000120725],"domain_scores_gemma":[0.99852717,0.00021891708,0.0006400743,0.00014526016,0.00017896858,0.0002895529],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005602684,0.00029710747,0.00030477362,0.002806964,0.00044764302,0.00071982347,0.0003918363,0.00027510384,0.0014258417],"category_scores_gemma":[0.0016351482,0.00021418734,0.0002491641,0.0011888162,0.00034876564,0.00029983494,0.0006381925,0.00023044166,0.00031467126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008298073,0.00003310452,0.9910936,0.0000074453033,0.000020180823,0.00012298767,0.00014012758,0.00004159391,0.0057651354,0.000027659626,0.0000761143,0.0025892104],"study_design_scores_gemma":[0.000003059449,0.00004339768,0.9989863,0.0000017998357,0.0000088667075,0.0002266757,0.0000864999,0.000110941364,0.0003570346,0.0000051186316,0.00016861854,0.0000017500059],"about_ca_topic_score_codex":0.010007739,"about_ca_topic_score_gemma":0.013274688,"teacher_disagreement_score":0.010007739,"about_ca_system_score_codex":0.00031246326,"about_ca_system_score_gemma":0.00022918417,"threshold_uncertainty_score":0.019898951},"labels":[],"label_agreement":null},{"id":"W4308579298","doi":"10.3847/1538-4357/ac9794","title":"A Quarter Century of Guitar Nebula/Filament Evolution","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Aeronautics and Space Administration","keywords":"Physics; Guitar; Quarter (Canadian coin); Astronomy; Protein filament; Astrophysics; Nebula; Astrobiology; Stars; Acoustics; Archaeology; History","score_opus":0.00766434801240435,"score_gpt":0.2099786426694597,"score_spread":0.20231429465705536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308579298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.86828005,0.08249866,0.0052738977,0.021113534,0.00092606444,0.000025593856,0.0012714567,0.00025179944,0.020358859],"genre_scores_gemma":[0.97097147,0.01679401,0.0022149326,0.0032286714,0.0007576619,0.000015267036,0.0005681298,0.00010529666,0.005344584],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99961084,0.000062775216,0.000024358904,0.0001747385,0.00006337765,0.00006395775],"domain_scores_gemma":[0.9986615,0.00041366447,0.00027614713,0.00023685576,0.00025862502,0.00015320715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014243495,0.00018226838,0.0003215895,0.00078713434,0.0007257316,0.002378444,0.00042526855,0.0011797813,0.00402536],"category_scores_gemma":[0.0031527036,0.0002556257,0.00019394666,0.00078481925,0.0020262876,0.0020431245,0.0011710402,0.001255335,0.00044649898],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017570213,0.00017735422,0.23086374,0.0009218103,0.00047771836,0.0023409096,0.01697411,0.0035339617,0.04739693,0.07509712,0.023272244,0.5971871],"study_design_scores_gemma":[0.00002845023,0.00030893038,0.495785,0.00046715318,0.00010072784,0.0020978665,0.0039314018,0.0020130705,0.008780981,0.0202952,0.46606636,0.0001248241],"about_ca_topic_score_codex":0.010789869,"about_ca_topic_score_gemma":0.007721993,"teacher_disagreement_score":0.010789869,"about_ca_system_score_codex":0.0021579126,"about_ca_system_score_gemma":0.00045665726,"threshold_uncertainty_score":0.021454155},"labels":[],"label_agreement":null},{"id":"W4308657423","doi":"10.3847/1538-4357/ac9796","title":"The Velocity Dispersion Function for Massive Quiescent and Star-forming Galaxies at 0.6 &lt; z ≤ 1.0","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Galaxy; Redshift; Sigma; Star formation; Astronomy; Star (game theory)","score_opus":0.0071972001703967834,"score_gpt":0.20063690100172962,"score_spread":0.19343970083133283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308657423","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957902,0.00016368304,0.00036979106,0.000038983424,0.00000399926,0.0000037703599,0.0017861348,0.00007150837,0.001771897],"genre_scores_gemma":[0.9976005,0.00003237576,0.00019456621,0.000013014443,0.0000069645944,0.0000021132273,0.0018285242,0.000009829599,0.0003121013],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998833,0.000008767229,0.0000055148134,0.000036032437,0.000027598113,0.00003878338],"domain_scores_gemma":[0.9989133,0.00014898303,0.00039855365,0.000083308834,0.00013500491,0.0003208347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032633185,0.00023055443,0.00021129506,0.002649097,0.00027965795,0.00077453174,0.00027151988,0.00031745128,0.0014108946],"category_scores_gemma":[0.00095291325,0.00011447224,0.00019875285,0.0008412075,0.00029537757,0.0004182314,0.00047400227,0.00023343368,0.00070524256],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007409142,0.00002119227,0.9840517,0.00001378672,0.000026386055,0.000038319642,0.0002717315,0.00029392447,0.0069092973,0.00033656982,0.000517876,0.0074450853],"study_design_scores_gemma":[0.0000014346024,0.000010539393,0.9989281,0.0000029222101,0.0000028178997,0.000028723312,0.000028759247,0.00026872617,0.00032900443,0.000061856736,0.0003342279,0.0000026743328],"about_ca_topic_score_codex":0.0049663438,"about_ca_topic_score_gemma":0.005604174,"teacher_disagreement_score":0.0049663438,"about_ca_system_score_codex":0.00035661826,"about_ca_system_score_gemma":0.00007670435,"threshold_uncertainty_score":0.00987488},"labels":[],"label_agreement":null},{"id":"W4308717995","doi":"10.3847/1538-4357/ac96f0","title":"Polarized Emission from Four Supernova Remnants in the THOR Survey","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"HORIZON EUROPE European Research Council; Natural Sciences and Engineering Research Council of Canada; Deutsche Forschungsgemeinschaft","keywords":"Physics; Faraday effect; Polarization (electrochemistry); Faraday cage; Astrophysics; Supernova; Stokes parameters; Optics; Magnetic field; Scattering","score_opus":0.023813069161422826,"score_gpt":0.24583892984073336,"score_spread":0.22202586067931052,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308717995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99958783,0.000016711128,0.000037613274,0.0000048467136,7.82346e-7,0.0000013332251,0.00013987266,0.000007710241,0.0002032664],"genre_scores_gemma":[0.9989158,0.000027200342,0.00010071477,0.0000099301,0.0000026904852,0.0000018018382,0.00077262614,0.0000059737317,0.00016327585],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998216,0.000026932934,0.000015385518,0.000042108768,0.000036308647,0.000057697373],"domain_scores_gemma":[0.9993654,0.00005344739,0.00020974649,0.00007879375,0.00008485288,0.00020776739],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032416225,0.00023189238,0.0002060241,0.0011772701,0.00034551133,0.0004742393,0.00017763585,0.00021718857,0.00074050634],"category_scores_gemma":[0.00044891986,0.00013900823,0.00032327682,0.00052920525,0.0003066018,0.00015503248,0.00069895503,0.00014588886,0.00030012606],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002756647,0.000031795804,0.9835169,0.00001170893,0.000073000774,0.00027168667,0.0003207112,0.0002551228,0.011980926,0.000058891896,0.00017594603,0.003027713],"study_design_scores_gemma":[0.000004758709,0.00004489566,0.99776053,0.0000026508922,0.000015889085,0.00028574688,0.00015654217,0.00020325833,0.0009610845,0.000015128915,0.0005452743,0.00000423594],"about_ca_topic_score_codex":0.0050320295,"about_ca_topic_score_gemma":0.0061087036,"teacher_disagreement_score":0.0050320295,"about_ca_system_score_codex":0.0002164518,"about_ca_system_score_gemma":0.00012332635,"threshold_uncertainty_score":0.010005474},"labels":[],"label_agreement":null},{"id":"W4308719048","doi":"10.3847/1538-4357/ac8c25","title":"New Coronae and Stellar Associations Revealed by a Clustering Analysis of the Solar Neighborhood","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"RES’EAU-WaterNET; National Aeronautics and Space Administration","keywords":"Physics; Exoplanet; Stars; Astrophysics; Open cluster; Stellar density; Astronomy; Star cluster","score_opus":0.00838618222506753,"score_gpt":0.2151407298989791,"score_spread":0.20675454767391155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308719048","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99892515,0.000038867973,0.00033420586,0.0000064243904,0.0000010444201,0.000006278317,0.00014743567,0.00001489782,0.00052557903],"genre_scores_gemma":[0.9990758,0.000012568335,0.00043953792,0.00000205454,0.0000018744944,0.0000025924924,0.00030348904,0.0000027118738,0.00015935945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980634,0.000016697446,0.000012953137,0.000065424225,0.00006710237,0.000031433963],"domain_scores_gemma":[0.99959046,0.00003708469,0.000099958066,0.00005617127,0.00012513984,0.00009124055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014308198,0.00009260657,0.00019407598,0.0020559113,0.000514761,0.00048520693,0.00019702151,0.00014122431,0.0008749345],"category_scores_gemma":[0.0005291473,0.000073915355,0.00018434056,0.0010261524,0.00021117985,0.0001595283,0.0004604637,0.000118949945,0.00025195722],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000108511,0.00004209465,0.96903294,0.000014489451,0.00006428856,0.0001667946,0.0004248884,0.00084165455,0.014992372,0.00019882352,0.00029815422,0.013815046],"study_design_scores_gemma":[0.0000014314732,0.000015116753,0.997122,0.0000017724647,0.000011769842,0.00012946485,0.00020223678,0.001499677,0.00059313595,0.000050672246,0.00036872318,0.00000405751],"about_ca_topic_score_codex":0.009399083,"about_ca_topic_score_gemma":0.010833109,"teacher_disagreement_score":0.009399083,"about_ca_system_score_codex":0.00026555467,"about_ca_system_score_gemma":0.00019461116,"threshold_uncertainty_score":0.018688738},"labels":[],"label_agreement":null},{"id":"W4308826295","doi":"10.3847/1538-4357/ac8f47","title":"Photometric Objects Around Cosmic Webs (PAC) Delineated in a Spectroscopic Survey. III. Accurate Measurement of Galaxy Stellar Mass Function with the Aid of Cosmological Redshift Surveys","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Max-Planck-Gesellschaft; National Natural Science Foundation of China; York University; Higher Education Discipline Innovation Project; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; Shanghai Jiao Tong University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Redshift; Astrophysics; Galaxy; Stellar mass; Sky; Measure (data warehouse); COSMIC cancer database; Astronomy; Star formation","score_opus":0.02210910741814426,"score_gpt":0.2255399893629015,"score_spread":0.20343088194475725,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4308826295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98322314,0.00019489884,0.0067254277,0.00002970553,0.0000101287305,0.000014027618,0.0012544416,0.00020064558,0.008347665],"genre_scores_gemma":[0.9951389,0.000055290806,0.0035048798,0.000009025064,0.000008292826,0.000010074045,0.00084229576,0.000019165516,0.00041197543],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99964035,0.000039949256,0.000023968401,0.00008998259,0.0001550368,0.000050666255],"domain_scores_gemma":[0.9988954,0.00009357398,0.00054141204,0.00021934227,0.00016634548,0.000083852865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004325523,0.00028323426,0.00020720948,0.0030368026,0.00027631118,0.0009385063,0.00022757912,0.000328407,0.00083197403],"category_scores_gemma":[0.0016980926,0.0002086695,0.00024080972,0.0021979515,0.00034439945,0.00097162835,0.0008064559,0.00021861776,0.00042662147],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009632962,0.000015959662,0.9465818,0.00003598243,0.00005464243,0.000099988,0.00020378962,0.0007579433,0.014113511,0.0027058779,0.0006572844,0.034676798],"study_design_scores_gemma":[0.000001361446,0.00001181283,0.9931369,0.000005473322,0.0000111380095,0.0001561759,0.000082319006,0.0021751553,0.002513217,0.0005126921,0.0013890836,0.0000047207022],"about_ca_topic_score_codex":0.0022583748,"about_ca_topic_score_gemma":0.0044901683,"teacher_disagreement_score":0.0030368026,"about_ca_system_score_codex":0.00033713275,"about_ca_system_score_gemma":0.00011572926,"threshold_uncertainty_score":0.004490435},"labels":[],"label_agreement":null},{"id":"W4309156261","doi":"10.3847/1538-4357/ac96ec","title":"Active Galactic Nuclei Continuum Reverberation Mapping Based on Zwicky Transient Facility Light Curves","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Deutsches Elektronen-Synchrotron; University of California, Irvine; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Ministério da Ciência, Tecnologia e Inovação; University of Portsmouth; Stockholms Universitet; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Ohio State University; National Research Foundation; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Science Foundation; National Research Foundation of Korea; New Mexico State University; Yale University; Vanderbilt University","keywords":"Physics; Light curve; Astrophysics; Transient (computer programming); Reverberation; Astronomy; Active galactic nucleus; Galaxy; Acoustics","score_opus":0.014365824515233157,"score_gpt":0.21950205208829604,"score_spread":0.20513622757306288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309156261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973826,0.000036511356,0.00058932276,0.0000052736273,5.034124e-7,0.000014068209,0.0013472696,0.000023977043,0.0006005706],"genre_scores_gemma":[0.99437547,0.000042325522,0.0013005568,0.000004478849,0.0000018468824,0.000022587607,0.0037501142,0.0000126159985,0.00048987305],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980944,0.00001579007,0.000011892911,0.00006200969,0.00005375942,0.000047067395],"domain_scores_gemma":[0.9989507,0.00011625553,0.0005063403,0.00012273317,0.0001715771,0.00013227484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025577296,0.00021587654,0.00015965887,0.00305046,0.0002373751,0.00040822773,0.00034646262,0.00010861742,0.0018133553],"category_scores_gemma":[0.00089123973,0.00010785511,0.000198841,0.0012808047,0.0001588339,0.0003345837,0.0005921916,0.00012278822,0.00051325496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037955855,0.000011303521,0.9837024,0.000008825804,0.00001952014,0.00005521238,0.00010691049,0.00034527987,0.0093178945,0.00006956069,0.00017780316,0.0061473744],"study_design_scores_gemma":[0.0000013839244,0.000014105814,0.9977176,0.000002869656,0.0000054900624,0.00004941066,0.00004775537,0.0005354587,0.0012753032,0.000013629137,0.00033438843,0.0000025881016],"about_ca_topic_score_codex":0.021508252,"about_ca_topic_score_gemma":0.050638605,"teacher_disagreement_score":0.021508252,"about_ca_system_score_codex":0.0004698701,"about_ca_system_score_gemma":0.0002881756,"threshold_uncertainty_score":0.042766094},"labels":[],"label_agreement":null},{"id":"W4309156393","doi":"10.3847/1538-4357/ac96f4","title":"Perfecting Our Set of Spectrophotometric Standard DA White Dwarfs","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Queen's University; European Commission; Queen's University Belfast; European Space Agency; National Aeronautics and Space Administration; U.S. Department of Energy; Nuclear Safety and Security Commission; Space Telescope Science Institute; Generalitat de Catalunya; National Science Foundation","keywords":"Physics; White dwarf; Observatory; Astrophysics; Light curve; Stars; Sky; Astronomy; Telescope","score_opus":0.015246857697494006,"score_gpt":0.24972295926957921,"score_spread":0.2344761015720852,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309156393","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9438658,0.00021201685,0.043513346,0.000108206674,0.00009504922,0.00022082267,0.0032480524,0.0008858983,0.007850787],"genre_scores_gemma":[0.951038,0.000053375763,0.04064483,0.000048418213,0.000035692297,0.0001481781,0.006050182,0.00013034549,0.0018509311],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9960891,0.000583344,0.00067741476,0.0010968337,0.0012677534,0.00028561527],"domain_scores_gemma":[0.97776365,0.0023639908,0.002273994,0.004853408,0.011902825,0.00084215763],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004674462,0.0006758883,0.0005900243,0.0037212137,0.0015117243,0.0017783645,0.0010309299,0.00048299198,0.0027253572],"category_scores_gemma":[0.014193008,0.00028041087,0.00044499736,0.0020568096,0.00053899235,0.0013988668,0.0012710807,0.00046686004,0.0019437575],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005007348,0.00023973767,0.83008057,0.00016090654,0.00011826636,0.00014497087,0.00057686516,0.004657584,0.03809624,0.0029660496,0.0027458658,0.11971214],"study_design_scores_gemma":[0.00009782749,0.0011769864,0.8036419,0.00008775725,0.00019454113,0.0006141996,0.0008813261,0.035337806,0.114286244,0.0024619985,0.041116707,0.00010273756],"about_ca_topic_score_codex":0.0074076126,"about_ca_topic_score_gemma":0.008466389,"teacher_disagreement_score":0.0074076126,"about_ca_system_score_codex":0.0010664958,"about_ca_system_score_gemma":0.0014955899,"threshold_uncertainty_score":0.024721205},"labels":[],"label_agreement":null},{"id":"W4309209386","doi":"10.3847/1538-4357/ac96eb","title":"Investigating the Effect of Galaxy Interactions on Star Formation at 0.5 &lt; z &lt; 3.0","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; NASA Exoplanet Science Institute; Nuclear Safety and Security Commission; W. M. Keck Foundation; Space Telescope Science Institute; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; California Institute of Technology; American Association for the Advancement of Science; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Star formation; Stellar mass; Active galactic nucleus; Universe; Galaxy formation and evolution; Bin; Astronomy","score_opus":0.008129251600004139,"score_gpt":0.22214326087147468,"score_spread":0.21401400927147055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309209386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987446,0.000013986979,0.00017327337,0.00002255313,0.0000010579379,0.0000014815528,0.00022370333,0.000028939105,0.0007904299],"genre_scores_gemma":[0.99955183,0.000005061982,0.00010001495,0.000006803656,0.0000012063115,0.0000011351198,0.00016547192,0.0000041227713,0.00016427865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999428,0.000006543374,0.0000017789203,0.000011344051,0.000011243487,0.000026301059],"domain_scores_gemma":[0.99945587,0.000094232484,0.00017230846,0.000029717525,0.00005611017,0.0001917302],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018215302,0.00010464572,0.00010842278,0.0003044899,0.000157971,0.00032235627,0.00014169358,0.00017893207,0.0017869379],"category_scores_gemma":[0.0004998694,0.00007539682,0.00020616263,0.00028817035,0.00016317442,0.00017897387,0.00024203637,0.00020472404,0.00028878122],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050757127,0.00011100261,0.9354663,0.00002590983,0.00008382698,0.00036306048,0.00022118664,0.0070221145,0.047555685,0.0009623402,0.0012310884,0.0064499225],"study_design_scores_gemma":[0.000004849822,0.00003563345,0.9927527,0.0000011792138,0.000009883365,0.000033628403,0.000051807267,0.0032252646,0.0035424614,0.000059615755,0.00027988132,0.0000031351258],"about_ca_topic_score_codex":0.007641624,"about_ca_topic_score_gemma":0.007385554,"teacher_disagreement_score":0.007641624,"about_ca_system_score_codex":0.00027509624,"about_ca_system_score_gemma":0.000107794964,"threshold_uncertainty_score":0.015194297},"labels":[],"label_agreement":null},{"id":"W4309300350","doi":"10.3847/1538-4357/ac9974","title":"COOL-LAMPS. II. Characterizing the Size and Star Formation History of a Bright Strongly Lensed Early-type Galaxy at Redshift 1.02","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Max-Planck-Gesellschaft; Brookhaven National Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; Office of Science; Fermilab; Max-Planck-Institut für Astronomie; Deutsche Forschungsgemeinschaft; Chinese Academy of Sciences; High Energy Physics; University of Sussex; University of Nottingham; Science and Technology Facilities Council; York University; University of Chicago; National Energy Research Scientific Computing Center; University of Michigan; National Science Foundation; Case Western Reserve University; Carnegie Mellon University; University of Cambridge; University of Pittsburgh; University of Arizona; Los Alamos National Laboratory; College of Engineering, Michigan State University; Princeton University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Universität Basel; SLAC National Accelerator Laboratory; Drexel University; Vanderbilt University; Harvard University; Ohio State University; University College London; National Aeronautics and Space Administration; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; Financiadora de Estudos e Projetos; University of Pennsylvania; New Mexico State University; University of Portsmouth; U.S. Department of Energy; Yale University; U.S. Naval Observatory; California Institute of Technology","keywords":"Physics; Astrophysics; Galaxy; Star formation; Astronomy; Stellar mass; Redshift; Fundamental plane (elliptical galaxies); Gravitational lens; Observatory; Billion years; Metallicity; Lenticular galaxy","score_opus":0.0091901921402479,"score_gpt":0.18907872485752658,"score_spread":0.17988853271727867,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309300350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99891186,0.000028633767,0.00014080801,0.000008086081,6.8046415e-7,0.0000020823732,0.0003427378,0.000027521648,0.0005375605],"genre_scores_gemma":[0.9985587,0.000016850805,0.00038927578,0.000008300091,0.0000024393964,0.0000019035906,0.0007280918,0.000011398986,0.00028312125],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999573,0.0000029851951,0.0000015362174,0.000012280314,0.000010880439,0.000014983094],"domain_scores_gemma":[0.99975437,0.000017391474,0.00008066669,0.000017042557,0.00002253246,0.000108014705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000115670795,0.00019197619,0.00016557933,0.0007835635,0.00024506252,0.00027873405,0.00017369246,0.00014168954,0.000999169],"category_scores_gemma":[0.00020372609,0.00014081647,0.00017560118,0.00033341066,0.00014315867,0.00017679065,0.0003181533,0.00012992584,0.000269455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022815762,0.000047235673,0.91746646,0.000030744988,0.000039732753,0.00038410668,0.00037493985,0.00087346515,0.06714775,0.0002252502,0.0006934,0.012488732],"study_design_scores_gemma":[0.000002500556,0.000026354286,0.9968587,0.0000016803347,0.000006013156,0.00015123426,0.000052509517,0.0009083016,0.0015584013,0.000025670583,0.00040509997,0.0000034255233],"about_ca_topic_score_codex":0.0103906235,"about_ca_topic_score_gemma":0.024344403,"teacher_disagreement_score":0.0103906235,"about_ca_system_score_codex":0.00037532515,"about_ca_system_score_gemma":0.00008932267,"threshold_uncertainty_score":0.020660281},"labels":[],"label_agreement":null},{"id":"W4309300381","doi":"10.3847/1538-4357/ac99de","title":"Multiwavelength Observations of the Obscuring Wind in the Radio-quiet Quasar MR 2251-178","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Quasar; Redshift; Astronomy; Active galactic nucleus; Galaxy; Supermassive black hole; Spectral line; Line-of-sight","score_opus":0.024293179506217594,"score_gpt":0.23452374419099392,"score_spread":0.21023056468477633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309300381","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989779,0.00008380782,0.000052648145,0.000010629596,0.000002277105,0.0000030539634,0.00021006244,0.000016860224,0.00064278644],"genre_scores_gemma":[0.99910814,0.000042260093,0.00019026503,0.000010577928,0.0000056453823,0.0000020157506,0.00029728145,0.0000027355525,0.0003410737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995136,0.0000028629975,0.0000030650574,0.00001582963,0.000013525901,0.000013318093],"domain_scores_gemma":[0.9998325,0.000007656741,0.0000730365,0.000010912582,0.00001797848,0.00005783799],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007980927,0.00015527851,0.00018604101,0.00069980754,0.0002846468,0.00026047535,0.00018122619,0.00012848439,0.00069067016],"category_scores_gemma":[0.000095817275,0.000103428465,0.00010005694,0.00027472718,0.000080741265,0.00010661404,0.0002267472,0.00021265283,0.00029122896],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002607624,0.00016745436,0.7781362,0.00006109507,0.000096884556,0.0032189237,0.00073614146,0.00016533276,0.19929639,0.00012781836,0.00085316616,0.016879864],"study_design_scores_gemma":[0.0000028608006,0.000051557974,0.9976216,0.0000021849046,0.000010119549,0.00045310913,0.00007679229,0.000096098265,0.0011118928,0.000007616429,0.0005638679,0.0000022334993],"about_ca_topic_score_codex":0.0037116036,"about_ca_topic_score_gemma":0.010794528,"teacher_disagreement_score":0.0037116036,"about_ca_system_score_codex":0.00014786045,"about_ca_system_score_gemma":0.000047919642,"threshold_uncertainty_score":0.0073800087},"labels":[],"label_agreement":null},{"id":"W4309309405","doi":"10.3847/1538-4357/ac9312","title":"Spinning up the Surface: Evidence for Planetary Engulfment or Unexpected Angular Momentum Transport?","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Horizon 2020 Framework Programme; University of Colorado Boulder; KU Leuven; Ministério da Ciência, Tecnologia e Inovação; Centre National d’Etudes Spatiales; Fonds De La Recherche Scientifique - FNRS; Deutsche Forschungsgemeinschaft; Vlaamse regering; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; European Commission; New Mexico State University; Fonds Wetenschappelijk Onderzoek; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University","keywords":"Physics; Angular momentum; Astrophysics; Rotation (mathematics); Stars; Planet; Astronomy; Envelope (radar); Stellar rotation; Luminosity; Stellar evolution; Classical mechanics; Geometry","score_opus":0.03406905575874625,"score_gpt":0.2674639941485276,"score_spread":0.23339493838978137,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309309405","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979594,0.00015308351,0.00048087296,0.0000654452,0.00000795771,0.0000018370915,0.00003551129,0.000026935533,0.0012688802],"genre_scores_gemma":[0.9995652,0.0000343089,0.00014939066,0.000018048857,0.000006873071,6.791614e-7,0.000040821782,0.000004872022,0.0001797644],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999484,0.000004597292,0.000003823952,0.00001433463,0.000012067492,0.000016846598],"domain_scores_gemma":[0.9996872,0.000055392335,0.00009903647,0.00006753836,0.000033491287,0.000057317695],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000107262895,0.000123192,0.00020458238,0.00043873198,0.000356486,0.000640947,0.00022819621,0.00041919152,0.002794697],"category_scores_gemma":[0.0005056573,0.000107394924,0.00010004072,0.0002873024,0.0005742367,0.0004629267,0.0005477494,0.0002797145,0.00061541353],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005295978,0.000064587475,0.5466518,0.00009831747,0.000044035085,0.0056109224,0.0005635566,0.00019365049,0.41934124,0.0011337033,0.00046034597,0.025308251],"study_design_scores_gemma":[0.00002625044,0.0003500975,0.9432815,0.000018548608,0.000040757408,0.010325332,0.0007277096,0.002076168,0.038347896,0.0014575626,0.0033311609,0.000017016435],"about_ca_topic_score_codex":0.0003618185,"about_ca_topic_score_gemma":0.0003478689,"teacher_disagreement_score":0.002794697,"about_ca_system_score_codex":0.0000919831,"about_ca_system_score_gemma":0.00005042905,"threshold_uncertainty_score":0.009349167},"labels":[],"label_agreement":null},{"id":"W4309374128","doi":"10.3847/1538-4357/ac952c","title":"CLASSY IV. Exploring UV Diagnostics of the Interstellar Medium in Local High-z Analogs at the Dawn of the JWST Era*","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":78,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Office of Science; Agencia Nacional de Investigación y Desarrollo; Leibniz-Institut für Astrophysik Potsdam; Space Telescope Science Institute; European Southern Observatory; Istituto Nazionale di Astrofisica; York University; Arizona Board of Regents; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Ministero dell’Istruzione, dell’Università e della Ricerca; Carnegie Mellon University; Leibniz-Gemeinschaft; Lorentz Center; University of Notre Dame; University of Arizona; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; University of Minnesota; National Science Foundation; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Physics; Interstellar medium; Astrochemistry; Astronomy; Astrobiology; Astrophysics; Galaxy","score_opus":0.014895445860658883,"score_gpt":0.20926049450484493,"score_spread":0.19436504864418605,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309374128","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99237835,0.0002161581,0.00077870634,0.00006390201,0.000008339333,0.000014667552,0.0025110317,0.0001337245,0.0038952194],"genre_scores_gemma":[0.99434966,0.00009619944,0.0016587876,0.000044881246,0.000017949375,0.00000969366,0.002922472,0.000048592057,0.00085177156],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989665,0.000006038693,0.0000036408098,0.000036244182,0.000028445755,0.000028846162],"domain_scores_gemma":[0.99947804,0.000037100963,0.00021049658,0.00006630015,0.000073267576,0.00013479493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028335472,0.0001647541,0.00015769558,0.0012572765,0.000311015,0.0009944314,0.00025099935,0.00019029934,0.0018826624],"category_scores_gemma":[0.0005318056,0.00010619115,0.00015070071,0.00083612575,0.00021270859,0.00050789426,0.0010041173,0.00024376078,0.0005467221],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008249209,0.00003839518,0.9634615,0.000039965737,0.000040447252,0.00018445773,0.00030751684,0.0004202022,0.008746553,0.0003863892,0.0016382122,0.024654023],"study_design_scores_gemma":[0.0000035013863,0.000013619258,0.99507755,0.000008003891,0.000007369214,0.00007110744,0.00021444717,0.00079684803,0.0011301837,0.00010966801,0.0025640205,0.0000036498939],"about_ca_topic_score_codex":0.0069310726,"about_ca_topic_score_gemma":0.012544773,"teacher_disagreement_score":0.0069310726,"about_ca_system_score_codex":0.0003178504,"about_ca_system_score_gemma":0.00016519376,"threshold_uncertainty_score":0.013781428},"labels":[],"label_agreement":null},{"id":"W4309391662","doi":"10.3847/1538-4357/ac983f","title":"The SDSS-Gaia View of the Color–Magnitude Relation for Blue Horizontal-branch Stars","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministério da Ciência, Tecnologia e Inovação; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Fundação de Amparo à Pesquisa do Estado de São Paulo; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Stars; Physics; Sky; Astrophysics; Surface gravity; Algorithm; Astronomy; Computer science","score_opus":0.009930235100894757,"score_gpt":0.22534890022987944,"score_spread":0.2154186651289847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309391662","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2698047,0.0042901486,0.11663468,0.002605382,0.0005563984,0.0002758667,0.3422376,0.09311888,0.17047636],"genre_scores_gemma":[0.6809551,0.0011647994,0.10224242,0.00092604087,0.00039677558,0.00024861615,0.18366005,0.007864961,0.022541173],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.99977463,0.000031334377,0.000013871911,0.000077221004,0.000058826867,0.000044059372],"domain_scores_gemma":[0.9992669,0.000085164414,0.00008392189,0.00021497613,0.00023566777,0.00011334],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000643313,0.00044930796,0.00032751026,0.0043967846,0.00030945186,0.0013758282,0.00032979978,0.0002694311,0.015494459],"category_scores_gemma":[0.001105366,0.0003077548,0.00046989674,0.0031498203,0.00012465645,0.0005586772,0.00078881334,0.00059521524,0.011288409],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067867787,0.00020344701,0.22642073,0.00040981988,0.0002102474,0.00024014419,0.0009064563,0.008677571,0.043334503,0.014719927,0.42860994,0.27558854],"study_design_scores_gemma":[0.000097330274,0.00007165244,0.59965974,0.000108685344,0.00007043979,0.00033979738,0.0002885025,0.019605996,0.007997159,0.007908969,0.36378458,0.000067110675],"about_ca_topic_score_codex":0.008717707,"about_ca_topic_score_gemma":0.012030718,"teacher_disagreement_score":0.015494459,"about_ca_system_score_codex":0.0003488303,"about_ca_system_score_gemma":0.00023783701,"threshold_uncertainty_score":0.051834166},"labels":[],"label_agreement":null},{"id":"W4309574089","doi":"10.3847/1538-4357/ac98c2","title":"Observations of 4U 1626–67 with the Imaging X-Ray Polarimetry Explorer","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"NASA Headquarters; Smithsonian Astrophysical Observatory; Russian Science Foundation; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Nuclear Safety and Security Commission; Academy of Finland; Marshall Space Flight Center; National Aeronautics and Space Administration; Goddard Space Flight Center; Smithsonian Institution","keywords":"Physics; Pulsar; Astrophysics; Polarimetry; Polarization (electrochemistry); Spectral line; Accretion (finance); Astronomy; Scattering; Optics","score_opus":0.017086102302267415,"score_gpt":0.2206597141732379,"score_spread":0.20357361187097048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309574089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978834,0.00015614959,0.00048661613,0.00001850495,0.000006241744,0.000007117875,0.00021006695,0.000026664185,0.0012053029],"genre_scores_gemma":[0.9978655,0.00008905738,0.0010180264,0.000022682974,0.000019713323,0.000007721556,0.00072910724,0.000013557985,0.00023474506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998436,0.0000307353,0.000008659061,0.000029842879,0.000051413856,0.0000357708],"domain_scores_gemma":[0.9995844,0.00007762833,0.00017439609,0.00005183648,0.00003660414,0.00007513447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048496737,0.00023390687,0.00030209887,0.00091318,0.00040297225,0.0004986321,0.00021301913,0.00029961005,0.00079030945],"category_scores_gemma":[0.0006205243,0.00021347459,0.00013842266,0.0006728984,0.00036546562,0.0002502791,0.0007677429,0.0004165787,0.0002829533],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014035107,0.00026403443,0.5786554,0.00016804367,0.00019143026,0.0016847686,0.0010403898,0.0020209714,0.38174415,0.0014103805,0.0009849658,0.030431923],"study_design_scores_gemma":[0.00005972986,0.0003624017,0.97123927,0.000030951913,0.00004634859,0.0010157505,0.00020845185,0.0020252932,0.021686645,0.0003148706,0.0029919478,0.000018425966],"about_ca_topic_score_codex":0.000645928,"about_ca_topic_score_gemma":0.0010762699,"teacher_disagreement_score":0.00091318,"about_ca_system_score_codex":0.00014915389,"about_ca_system_score_gemma":0.00010434379,"threshold_uncertainty_score":0.0026438236},"labels":[],"label_agreement":null},{"id":"W4309603942","doi":"10.3847/1538-4357/ac940b","title":"Spacetime Metrics and Ringdown Waveforms for Galactic Black Holes Surrounded by a Dark Matter Spike","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Dark matter; Spike (software development); Astrophysics; Astronomy; Spacetime; Black hole (networking); Universe; Quantum mechanics","score_opus":0.008110266402114754,"score_gpt":0.21303639342147965,"score_spread":0.20492612701936488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309603942","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9370603,0.00028880883,0.05020372,0.0006229499,0.000054655833,0.000037101036,0.00026429546,0.00027453565,0.011193589],"genre_scores_gemma":[0.99200046,0.000101847625,0.0056683337,0.00003438982,0.000027104832,0.0000100259485,0.00019882062,0.000045800625,0.0019132898],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992347,0.000021982813,0.000004849724,0.000014685008,0.00001974057,0.000015206892],"domain_scores_gemma":[0.99942493,0.0000684246,0.00016946284,0.00003939079,0.00010909284,0.00018868851],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029058108,0.00045549215,0.00023227144,0.0008874218,0.000384428,0.0007607192,0.00043219907,0.0005634653,0.0037982087],"category_scores_gemma":[0.0015853884,0.00017885854,0.00029819403,0.0002302124,0.0006452725,0.0011242379,0.0008459214,0.00048394754,0.00036505386],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034998782,0.000046662528,0.009768554,0.00007783065,0.00003637507,0.0022342228,0.0007867494,0.04499143,0.028662099,0.8943649,0.0031338916,0.0155471545],"study_design_scores_gemma":[0.00007763671,0.00018104332,0.020986732,0.00003893691,0.000018253138,0.00096235645,0.00046234447,0.54540247,0.0039125523,0.42207104,0.0057806564,0.00010595581],"about_ca_topic_score_codex":0.0014775335,"about_ca_topic_score_gemma":0.00079387054,"teacher_disagreement_score":0.0037982087,"about_ca_system_score_codex":0.00063451636,"about_ca_system_score_gemma":0.00014945997,"threshold_uncertainty_score":0.01270628},"labels":[],"label_agreement":null},{"id":"W4309675532","doi":"10.3847/1538-4357/ac94ce","title":"Structure in the Magnetic Field of the Milky Way Disk and Halo Traced by Faraday Rotation","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan College; University of Calgary; Okanagan University College; University of British Columbia, Okanagan Campus; Canadian Institute for Theoretical Astrophysics; National Research Council Canada; University of British Columbia; Dominion Astrophysical Observatory; University of Toronto","funders":"HORIZON EUROPE Marie Sklodowska-Curie Actions; University of Toronto; European Commission; Natural Sciences and Engineering Research Council of Canada; Hrvatska Zaklada za Znanost; National Natural Science Foundation of China","keywords":"Physics; Faraday effect; Milky Way; Astrophysics; Galaxy; Rotation (mathematics); Magnetic field; Geometry; Mathematics","score_opus":0.004433717762183787,"score_gpt":0.2010025404266197,"score_spread":0.1965688226644359,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309675532","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986563,0.00009629055,0.000051830004,0.000019472822,0.0000010593445,9.082752e-7,0.00024769545,0.0000134962,0.0009129613],"genre_scores_gemma":[0.99903643,0.0000516368,0.000053730306,0.0000075630696,0.0000036693318,0.0000014401757,0.0004985587,0.000007981401,0.000339048],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999331,0.000010822885,0.00000409018,0.00001972029,0.000013764763,0.000018523802],"domain_scores_gemma":[0.99939823,0.00009774021,0.00020789017,0.000043634656,0.00010367427,0.0001488508],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012959733,0.00008183961,0.00015756633,0.0014292403,0.00012869995,0.00061897736,0.000115235496,0.0001416301,0.0015840884],"category_scores_gemma":[0.0009161172,0.00008227561,0.00014280951,0.0008995553,0.00023836893,0.00026789345,0.00043205346,0.00008901028,0.0004069479],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016549358,0.000013017288,0.98257655,0.000022774917,0.0000627556,0.00009249361,0.0005465722,0.0003583476,0.00766871,0.00024064527,0.00039199326,0.0078605665],"study_design_scores_gemma":[0.0000022406443,0.0000074911277,0.9993709,0.0000030060266,0.0000041373373,0.000020231892,0.00009019921,0.00009649261,0.00012410224,0.000032342836,0.00024695488,0.0000020383677],"about_ca_topic_score_codex":0.00949292,"about_ca_topic_score_gemma":0.010573317,"teacher_disagreement_score":0.00949292,"about_ca_system_score_codex":0.00026138214,"about_ca_system_score_gemma":0.00008927976,"threshold_uncertainty_score":0.01887536},"labels":[],"label_agreement":null},{"id":"W4309736345","doi":"10.3847/1538-4357/ac940a","title":"Distances, Radial Distribution, and Total Number of Galactic Supernova Remnants","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Supernova; Astrophysics; Galaxy; Galaxy rotation curve; Range (aeronautics); Molecular cloud; Maser; Selection (genetic algorithm); Stars; Galaxy formation and evolution","score_opus":0.006017455287421247,"score_gpt":0.22052751385144986,"score_spread":0.2145100585640286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309736345","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933021,0.00066675973,0.0008001606,0.000017123244,0.000003852081,0.0000072908824,0.002371677,0.00008827973,0.0027426824],"genre_scores_gemma":[0.99400854,0.00036949856,0.0007080287,0.000007837705,0.0000067661695,0.000006792094,0.0037934312,0.000017315298,0.0010817806],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995784,0.000060930222,0.000097159274,0.00010219357,0.000112569665,0.0000487505],"domain_scores_gemma":[0.9982685,0.0005075524,0.00043888172,0.00027220708,0.00035244628,0.00016038056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00075346953,0.00022352823,0.00026632423,0.0024826922,0.00022874713,0.00064562185,0.00033203748,0.00013074573,0.002350684],"category_scores_gemma":[0.0028133767,0.00011346503,0.00032011146,0.00088895235,0.00026094215,0.00037286745,0.00039480682,0.00010810862,0.00072428066],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001631814,0.00001468232,0.9809686,0.00003194792,0.00013111868,0.000108479595,0.000056779187,0.0014119163,0.0016960811,0.00053214247,0.00038000036,0.014505048],"study_design_scores_gemma":[0.0000068680015,0.00013513956,0.98992234,0.000014765454,0.00007828658,0.0012504156,0.00011342263,0.002067189,0.0028776305,0.00032367292,0.0031940928,0.000016093165],"about_ca_topic_score_codex":0.00235141,"about_ca_topic_score_gemma":0.0021362843,"teacher_disagreement_score":0.0024826922,"about_ca_system_score_codex":0.00022177155,"about_ca_system_score_gemma":0.0001203666,"threshold_uncertainty_score":0.00786382},"labels":[],"label_agreement":null},{"id":"W4309736778","doi":"10.3847/1538-4357/ac9972","title":"Simulated Bars May Be Shorter but Are Not Slower Than Those Observed: TNG50 versus MaNGA","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Galaxy; Context (archaeology); Bar (unit); Galaxy formation and evolution; Stellar mass; Star formation","score_opus":0.029668817109875803,"score_gpt":0.2420054048988894,"score_spread":0.2123365877890136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4309736778","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99656373,0.000029912047,0.00078060245,0.0000876771,0.000007767742,0.0000040927816,0.00062591437,0.0001431256,0.0017572787],"genre_scores_gemma":[0.99856204,0.000009404873,0.0005275701,0.000023408784,0.0000021222736,0.000004272266,0.00066423154,0.00003756174,0.00016933866],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983823,0.000040461964,0.000008879646,0.000055690405,0.00002089803,0.000035880897],"domain_scores_gemma":[0.9988663,0.00054317224,0.00012244679,0.0001692614,0.000119413824,0.00017947434],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004770235,0.00022867255,0.00023154421,0.0003217376,0.00025893422,0.000733092,0.0005415528,0.00038274867,0.0023215339],"category_scores_gemma":[0.0026442346,0.00014478037,0.0002519798,0.00043905515,0.0004220504,0.00042743256,0.000357855,0.00037615816,0.00018661575],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000742586,0.0002150311,0.40320924,0.000091129295,0.00027399996,0.00035777665,0.0003261471,0.561831,0.012311129,0.0065257237,0.0046910015,0.009425265],"study_design_scores_gemma":[0.00014696096,0.00015890785,0.1884712,0.000021509817,0.00007786541,0.00011773493,0.00029159596,0.7982012,0.007220773,0.0026256968,0.0026216533,0.00004483561],"about_ca_topic_score_codex":0.01397541,"about_ca_topic_score_gemma":0.01034112,"teacher_disagreement_score":0.01397541,"about_ca_system_score_codex":0.0005732201,"about_ca_system_score_gemma":0.00025776005,"threshold_uncertainty_score":0.027788103},"labels":[],"label_agreement":null},{"id":"W4310290428","doi":"10.3847/1538-4357/ac9bfc","title":"Variability from Thermoresistive Instability in the Atmospheres of Hot Jupiters","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Instability; Physics; Jupiter (rocket family); Electrical resistivity and conductivity; Magnetohydrodynamics; Hot Jupiter; Oscillation (cell signaling); Atmosphere (unit); Joule heating; Zonal flow (plasma); Astrophysics; Mechanics; Magnetic field; Thermodynamics; Planet; Plasma; Astronomy; Chemistry; Tokamak","score_opus":0.007147428140795131,"score_gpt":0.21350103073934004,"score_spread":0.2063536025985449,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310290428","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980761,0.00015867251,0.0010733833,0.000047482783,0.000002100404,0.0000023221342,0.00003293842,0.000023364635,0.0005836231],"genre_scores_gemma":[0.9996351,0.000056073313,0.00016821681,0.000005860194,0.0000026001778,0.0000015631633,0.00002996889,0.0000024195629,0.00009816155],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99997425,0.000005190328,0.0000015896958,0.000007709913,0.000006526217,0.000004723063],"domain_scores_gemma":[0.99994266,0.000009759366,0.000027292153,0.0000058558735,0.0000042839547,0.0000101708165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000060529375,0.00022993777,0.00018640964,0.00018603393,0.00021869928,0.0005612693,0.00023087757,0.0002932252,0.00049098185],"category_scores_gemma":[0.00021885199,0.00011740152,0.00017809172,0.0001498967,0.00045480012,0.00027191834,0.000340217,0.00020689242,0.000075819684],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027698383,0.00004818543,0.044195,0.00014514483,0.000081952734,0.0009938792,0.0004634476,0.08650868,0.85553604,0.0062446566,0.0002763445,0.0052295947],"study_design_scores_gemma":[0.00012109539,0.0005732139,0.4424097,0.00003233526,0.000083729115,0.0014297497,0.0004329472,0.43330926,0.09361231,0.023131786,0.004803912,0.000059974922],"about_ca_topic_score_codex":0.0010116777,"about_ca_topic_score_gemma":0.00048353,"teacher_disagreement_score":0.0010116777,"about_ca_system_score_codex":0.0002636995,"about_ca_system_score_gemma":0.00006766809,"threshold_uncertainty_score":0.0020115376},"labels":[],"label_agreement":null},{"id":"W4310291202","doi":"10.3847/1538-4357/ac997b","title":"Proper Motions, Orbits, and Tidal Influences of Milky Way Dwarf Spheroidal Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":117,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Fermilab; High Energy Physics; Natural Sciences and Engineering Research Council of Canada; Office of Science; Division of Astronomical Sciences; Institut de Física d'Altes Energies; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; Deutsche Forschungsgemeinschaft; Ohio State University; Science and Technology Facilities Council; University College London; National Science Foundation; European Space Agency; Argonne National Laboratory; U.S. Department of Energy; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University of Chicago","keywords":"Physics; Astrophysics; Milky Way; Local Group; Astrometry; Astronomy; Proper motion; Galaxy; Orbital elements; Photometry (optics); Large Magellanic Cloud; Stars","score_opus":0.011180052524473426,"score_gpt":0.21776545737719996,"score_spread":0.20658540485272653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310291202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990023,0.000025258872,0.0005815112,0.000012770736,9.368739e-7,0.000001689496,0.000091499074,0.000021862443,0.00026222062],"genre_scores_gemma":[0.9994824,0.000012262933,0.00025526687,0.0000024777796,0.0000010668775,0.0000012125366,0.00015926475,0.000005245924,0.00008072261],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998983,0.00002593918,0.0000066364823,0.000030371124,0.000023328359,0.00001532332],"domain_scores_gemma":[0.99952745,0.0001641608,0.00011555729,0.00006982817,0.00005207641,0.00007091997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040730395,0.00015871687,0.00021656946,0.00051636354,0.00020674827,0.00047141674,0.00032708124,0.00019165357,0.0006815442],"category_scores_gemma":[0.0018156284,0.00027195332,0.00046307963,0.0004113076,0.00023749303,0.0004197315,0.00041283335,0.00013288979,0.00014000366],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013032458,0.00002638791,0.8047319,0.000011157724,0.0001445218,0.00009958665,0.00009412817,0.18663861,0.002375355,0.00093048456,0.00018970328,0.0046279137],"study_design_scores_gemma":[0.00003797631,0.00009209135,0.5464482,0.00000955839,0.000057790938,0.00008688653,0.00012159677,0.44989356,0.0015545087,0.0010124593,0.0006628245,0.000022574823],"about_ca_topic_score_codex":0.014746796,"about_ca_topic_score_gemma":0.012633058,"teacher_disagreement_score":0.014746796,"about_ca_system_score_codex":0.00050216867,"about_ca_system_score_gemma":0.00022643608,"threshold_uncertainty_score":0.029321909},"labels":[],"label_agreement":null},{"id":"W4310291405","doi":"10.3847/1538-4357/ac9b4b","title":"A Ghost in Boötes: The Least-Luminous Disrupted Dwarf Galaxy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Metallicity; Dwarf galaxy; Galaxy; Surface brightness; Luminosity; Stars; Astrometry; Astronomy","score_opus":0.010691316328817388,"score_gpt":0.2244658569008457,"score_spread":0.2137745405720283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310291405","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9942526,0.00022363811,0.0009960751,0.00016913998,0.000025339863,0.00000574397,0.00021844149,0.00019430183,0.0039145863],"genre_scores_gemma":[0.997174,0.000036020443,0.0008829977,0.000060640243,0.0000194554,0.0000011915125,0.0003023119,0.000030847903,0.0014923967],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987257,0.000008761484,0.0000052833702,0.000045916444,0.000034723602,0.0000328517],"domain_scores_gemma":[0.9994759,0.00005400402,0.000116114046,0.00013179184,0.000040362447,0.00018174513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001734864,0.0002148099,0.00023507352,0.00056410127,0.00052720093,0.000749097,0.00025371867,0.00034080422,0.002849537],"category_scores_gemma":[0.00059135177,0.00014232758,0.00012792765,0.000231382,0.00073955883,0.00055430026,0.0009456006,0.00028780464,0.0008374657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000985465,0.00018524921,0.6771469,0.00011833742,0.00007441252,0.01310247,0.0042974046,0.00068694924,0.20749648,0.014695273,0.010042587,0.07116859],"study_design_scores_gemma":[0.00007099975,0.0006463038,0.786284,0.00006291117,0.00006554353,0.042815663,0.0024277351,0.004293789,0.052319594,0.010131392,0.10080865,0.00007333572],"about_ca_topic_score_codex":0.0012518622,"about_ca_topic_score_gemma":0.0018383072,"teacher_disagreement_score":0.002849537,"about_ca_system_score_codex":0.0002761579,"about_ca_system_score_gemma":0.000109873625,"threshold_uncertainty_score":0.00953269},"labels":[],"label_agreement":null},{"id":"W4310291831","doi":"10.3847/1538-4357/ac9af1","title":"The Correlation between WISE 12 μm Emission and Molecular Gas Tracers on Subkiloparsec Scales in Nearby Star-forming Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Galaxy; Star formation; Isotopologue; Luminosity; Trace gas; Molecular cloud; Astronomy; Stars; Spectral line","score_opus":0.007449321186266456,"score_gpt":0.20998819348139597,"score_spread":0.2025388722951295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310291831","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99930334,0.000043112253,0.00015995261,0.000011547778,8.5033514e-7,0.0000012824443,0.00014676819,0.000013634107,0.00031948282],"genre_scores_gemma":[0.9996136,0.000016955377,0.00013011158,0.0000052453775,0.0000022398508,0.0000018737908,0.0001591458,0.0000029318383,0.00006789897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998715,0.000015672886,0.00000643266,0.00005473933,0.000024034953,0.000027563961],"domain_scores_gemma":[0.9988237,0.00020278836,0.0005228522,0.00014891627,0.00010725566,0.00019445417],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026237764,0.00017249919,0.00021964028,0.00092801696,0.00018135636,0.00047777322,0.00020570219,0.00017814623,0.0011261913],"category_scores_gemma":[0.001267245,0.00017681695,0.0001711872,0.00059641036,0.00027878745,0.0003618416,0.0005552634,0.00020644098,0.00026631582],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000045639623,0.000013019206,0.9894338,0.000007382106,0.00003774115,0.000025903144,0.000104029314,0.00016180897,0.007823931,0.000083491104,0.00005554037,0.0022076007],"study_design_scores_gemma":[5.8530725e-7,0.000005301234,0.99959356,7.689134e-7,0.000003064475,0.000010523706,0.000026711463,0.00014626466,0.00014420883,0.00001925981,0.000048983788,8.0571294e-7],"about_ca_topic_score_codex":0.0035374947,"about_ca_topic_score_gemma":0.0055689425,"teacher_disagreement_score":0.0035374947,"about_ca_system_score_codex":0.000174793,"about_ca_system_score_gemma":0.00008825646,"threshold_uncertainty_score":0.007033825},"labels":[],"label_agreement":null},{"id":"W4310478548","doi":"10.3847/1538-4357/ac9b47","title":"Probing Accretion Turbulence in the Galactic Center with EHT Polarimetry","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada; Innovation, Science and Economic Development Canada; Institut Périmètre de physique théorique; University of Illinois at Urbana-Champaign; Government of Canada; Ministero dello Sviluppo Economico","keywords":"Physics; Galactic Center; Astrophysics; Polarimetry; Astronomy; Accretion (finance); Turbulence; Accretion disc; Stars; Scattering; Optics","score_opus":0.010942575280302591,"score_gpt":0.22215458660698087,"score_spread":0.21121201132667827,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310478548","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98502535,0.00004751166,0.011609018,0.000065985936,0.000012686987,0.00002001362,0.00047400148,0.00016454367,0.0025809025],"genre_scores_gemma":[0.99247324,0.000022370024,0.007027152,0.000015699385,0.000012269223,0.000005388698,0.0003050494,0.000012229808,0.00012661533],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998666,0.000029832836,0.000003372654,0.000031657888,0.00003920076,0.000029374889],"domain_scores_gemma":[0.99978286,0.000045111035,0.000054564887,0.00003890973,0.000045248824,0.000033218475],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003678998,0.0002541169,0.00020195972,0.0005864576,0.00024676046,0.00057981035,0.00020257049,0.00018938287,0.0006295869],"category_scores_gemma":[0.00046517228,0.00012200322,0.00015620085,0.00051010837,0.0002884744,0.00029817928,0.0004577968,0.0002779072,0.00015422126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014937508,0.000451212,0.39615792,0.00007361549,0.00020942245,0.00035669238,0.00023645075,0.12308599,0.3894574,0.0051171337,0.001686664,0.08167374],"study_design_scores_gemma":[0.0001768915,0.00035348552,0.4314836,0.000019277984,0.000074234245,0.00018126465,0.00016916312,0.475121,0.08816948,0.0025039476,0.0016837376,0.00006395048],"about_ca_topic_score_codex":0.0022828053,"about_ca_topic_score_gemma":0.0036947115,"teacher_disagreement_score":0.0022828053,"about_ca_system_score_codex":0.0002508615,"about_ca_system_score_gemma":0.00023832757,"threshold_uncertainty_score":0.004539013},"labels":[],"label_agreement":null},{"id":"W4310808865","doi":"10.3847/1538-4357/ac9cda","title":"Rocky Histories: The Effect of High Excitations on the Formation of Rocky Planets","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrobiology; Planet; Astronomy","score_opus":0.005781402371279172,"score_gpt":0.19304329593692818,"score_spread":0.187261893565649,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310808865","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959973,0.000084252,0.0009429322,0.00013996002,0.000013201797,0.000007955588,0.0001293894,0.00007288636,0.0026122828],"genre_scores_gemma":[0.99929523,0.000020012048,0.00042111473,0.000021091468,0.0000017685219,0.0000039297634,0.000053460102,0.00002386922,0.00015946242],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997571,0.00006963591,0.000012534972,0.00004482854,0.000039551618,0.00007632227],"domain_scores_gemma":[0.99731797,0.0017038339,0.00029565362,0.00017399453,0.0001311785,0.00037738768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056706916,0.00029872757,0.00027310336,0.0004003156,0.0008290653,0.0010337229,0.0007430653,0.0006246277,0.002727953],"category_scores_gemma":[0.0057324744,0.00030903495,0.00032477535,0.00027216162,0.00084126764,0.0007676551,0.00094017904,0.0008861763,0.00017638452],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040158295,0.00025960582,0.13146831,0.00009502957,0.0001670844,0.00075577747,0.00022245196,0.84412885,0.010461102,0.003977845,0.0013390963,0.0067232577],"study_design_scores_gemma":[0.00008739994,0.00043426108,0.04942618,0.000045818822,0.00008777541,0.00021486741,0.00053580786,0.934623,0.010806027,0.0019732572,0.0017137857,0.000051828054],"about_ca_topic_score_codex":0.0069939233,"about_ca_topic_score_gemma":0.0066751507,"teacher_disagreement_score":0.0069939233,"about_ca_system_score_codex":0.0006879761,"about_ca_system_score_gemma":0.00049579085,"threshold_uncertainty_score":0.013906419},"labels":[],"label_agreement":null},{"id":"W4310848126","doi":"10.3847/1538-4357/ac9cd9","title":"A New Distance to the Supernova Remnant DA 530 Based on H i Absorption of Polarized Emission","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Brandon University; University of Calgary","funders":"","keywords":"Physics; Astrophysics; Galactic plane; Interstellar medium; Absorption (acoustics); Supernova; Observatory; Supernova remnant; Milky Way; Astronomy; Galaxy; Optics","score_opus":0.009542159359744054,"score_gpt":0.22582635334187076,"score_spread":0.2162841939821267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310848126","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99659413,0.00017986793,0.00074495905,0.000036902828,0.000008989255,0.0000050241397,0.00031758405,0.000067746514,0.0020447571],"genre_scores_gemma":[0.9985318,0.00003622959,0.0008200693,0.000017322249,0.000005084613,0.0000025680179,0.00035259977,0.00000841795,0.00022584942],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999201,0.0000053047006,0.000007906333,0.000037471258,0.000014052165,0.000015106499],"domain_scores_gemma":[0.99958724,0.000039563114,0.00016756367,0.00003119851,0.00006476632,0.00010959476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000131385,0.0002762414,0.00020862155,0.0006719931,0.00031059896,0.0008294371,0.00023165283,0.00035872587,0.001895476],"category_scores_gemma":[0.00037305817,0.00015559226,0.00022099605,0.00027549127,0.0002188355,0.00025413968,0.00043300592,0.000364649,0.0006025284],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062839204,0.000053799195,0.83100224,0.000058905513,0.00007787758,0.0014182753,0.0002635374,0.00047311359,0.15330453,0.00078326726,0.0006848929,0.011251181],"study_design_scores_gemma":[0.000013623653,0.000107685315,0.98249674,0.000013542614,0.0000652487,0.0019513319,0.0002056876,0.0014149563,0.011289103,0.00022314937,0.002202313,0.000016730968],"about_ca_topic_score_codex":0.0052028582,"about_ca_topic_score_gemma":0.0063075675,"teacher_disagreement_score":0.0052028582,"about_ca_system_score_codex":0.00042145234,"about_ca_system_score_gemma":0.00011599619,"threshold_uncertainty_score":0.010345161},"labels":[],"label_agreement":null},{"id":"W4310848131","doi":"10.3847/1538-4357/ac9c64","title":"The Anisotropic Circumgalactic Medium of Massive Early-type Galaxies","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Office of Science; Johns Hopkins University; Carnegie Mellon University; College of Engineering, Michigan State University; Harvard University; Huazhong University of Science and Technology; Ohio State University; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Galaxy; Intergalactic medium; Astrophysics; Astronomy; Anisotropy; Quasar; Optics; Redshift","score_opus":0.007514024828883471,"score_gpt":0.21042503842226787,"score_spread":0.2029110135933844,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310848131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990652,0.000097445045,0.00024680543,0.000008655125,0.0000011658128,0.0000012364308,0.00005344158,0.0000074109976,0.0005186716],"genre_scores_gemma":[0.9998317,0.00002347539,0.000072672236,0.0000038050666,0.0000015326442,3.0127418e-7,0.00003749969,8.490065e-7,0.000028131377],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992955,0.000012239566,0.0000032383346,0.00002184962,0.00001620774,0.000016925831],"domain_scores_gemma":[0.99948585,0.00007199863,0.00025022516,0.000049147053,0.000033653352,0.00010916027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015238847,0.00022038897,0.00015938871,0.0007657993,0.00017531459,0.0007254937,0.00019197968,0.000120559365,0.00057705375],"category_scores_gemma":[0.0004937664,0.00014541276,0.00008607572,0.00032892652,0.00046110363,0.00028292605,0.0004733848,0.00016044971,0.000121190074],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003065937,0.000020088466,0.87286973,0.000025977028,0.000056740177,0.00027316654,0.00023944389,0.0004332466,0.1204099,0.00042616547,0.000067139255,0.0048718895],"study_design_scores_gemma":[0.0000038032183,0.00001885674,0.99544525,0.0000023834093,0.0000103669,0.00015655784,0.00010675717,0.00038559627,0.0035698013,0.00012838391,0.00016944688,0.000002776244],"about_ca_topic_score_codex":0.0035367936,"about_ca_topic_score_gemma":0.0040210667,"teacher_disagreement_score":0.0035367936,"about_ca_system_score_codex":0.00020534574,"about_ca_system_score_gemma":0.000080900805,"threshold_uncertainty_score":0.0070323944},"labels":[],"label_agreement":null},{"id":"W4310878017","doi":"10.3847/1538-4357/ac9cd0","title":"Millisecond Pulsars in Dense Star Clusters: Evolution, Scaling Relations, and the Galactic-center Gamma-Ray Excess","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; National Science Foundation","keywords":"Globular cluster; Physics; Millisecond pulsar; Astrophysics; Milky Way; Galactic Center; Astronomy; Star cluster; Pulsar; Population; Cluster (spacecraft); Galaxy","score_opus":0.007598008733752337,"score_gpt":0.21781246402274818,"score_spread":0.21021445528899585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4310878017","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99834514,0.00004038443,0.0011930321,0.000026575437,0.0000014750192,0.00000240657,0.000043157506,0.000017920653,0.00033000964],"genre_scores_gemma":[0.999432,0.000026463118,0.0003959302,0.000004318725,0.0000013935013,0.0000025888721,0.00005378881,0.000006229304,0.00007719667],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999416,0.000015318621,0.0000032085484,0.00001698062,0.000011648026,0.000011250713],"domain_scores_gemma":[0.9989736,0.00053188344,0.00025368918,0.00007512552,0.00007124283,0.00009450021],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006235523,0.0002720781,0.00022475533,0.0004842041,0.00030552046,0.0006112899,0.00035449397,0.00036328138,0.00053472037],"category_scores_gemma":[0.0031099294,0.00019700744,0.00030391564,0.00034985144,0.0004813505,0.0004868952,0.000431469,0.0002416059,0.00007330425],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009583028,0.00007421981,0.37232313,0.000035771067,0.0001061632,0.00021982857,0.0001858888,0.6101536,0.007263464,0.005223429,0.00028350603,0.0040351846],"study_design_scores_gemma":[0.00001853582,0.000036337744,0.088301,0.0000064446936,0.000022952641,0.000058338872,0.00005793298,0.9068291,0.0018265217,0.0026757438,0.00015528055,0.000011823822],"about_ca_topic_score_codex":0.006941872,"about_ca_topic_score_gemma":0.0042059766,"teacher_disagreement_score":0.006941872,"about_ca_system_score_codex":0.0006884798,"about_ca_system_score_gemma":0.00021330612,"threshold_uncertainty_score":0.013802946},"labels":[],"label_agreement":null},{"id":"W4311007143","doi":"10.3847/1538-4357/ac9df5","title":"Measuring He i Stark Line Shapes in the Laboratory to Examine Differences in Photometric and Spectroscopic DB White Dwarf Masses","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Ministerio de Ciencia e Innovación; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Stark effect; White dwarf; Line (geometry); Astrophysics; Helium; van der Waals force; Spectral line; Computational physics; Stars; Atomic physics; Astronomy; Quantum mechanics","score_opus":0.025434935027683545,"score_gpt":0.24287017716546144,"score_spread":0.2174352421377779,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311007143","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9903167,0.000086022796,0.007367768,0.000032675925,0.000013832744,0.000015521544,0.00034239556,0.00022420078,0.0016009395],"genre_scores_gemma":[0.9952034,0.00003515094,0.0037580933,0.000053604814,0.0000042331017,0.000013661805,0.00028262695,0.000033773198,0.00061550253],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9998134,0.000019573627,0.000010333066,0.000077783225,0.00005737109,0.000021541136],"domain_scores_gemma":[0.9997004,0.00004834239,0.000078638994,0.000044489632,0.000077026474,0.000051113137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003896889,0.00017356696,0.00011524988,0.00033350603,0.0002800705,0.00039899678,0.00030220172,0.00031969426,0.0011265879],"category_scores_gemma":[0.00052836706,0.00011004056,0.00012846147,0.00017536558,0.00021163339,0.00038204362,0.00046721825,0.00032237748,0.00048953295],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002327898,0.0001264597,0.17439812,0.0000418215,0.000047680554,0.00007873364,0.00034716804,0.00070475054,0.81208146,0.0003628731,0.00036856259,0.011209581],"study_design_scores_gemma":[0.00001394266,0.00058961206,0.39465716,0.00001434311,0.00005056186,0.0003100438,0.0006061735,0.006571031,0.59279805,0.00039828545,0.003960136,0.000030773903],"about_ca_topic_score_codex":0.0008496495,"about_ca_topic_score_gemma":0.0016729055,"teacher_disagreement_score":0.0011265879,"about_ca_system_score_codex":0.00020551261,"about_ca_system_score_gemma":0.000100868165,"threshold_uncertainty_score":0.0037688017},"labels":[],"label_agreement":null},{"id":"W4311101691","doi":"10.3847/1538-4357/ace902","title":"Target Selection and Sample Characterization for the DESI LOW-Z Secondary Target Program","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"U.S. Department of Energy; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Surface brightness; Universe; Sky; Dark energy; Astronomy; Cosmology","score_opus":0.008152307980202294,"score_gpt":0.22374401338587757,"score_spread":0.21559170540567527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311101691","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9335378,0.00012877131,0.024465458,0.00022443877,0.000022683926,0.00037506572,0.023034446,0.0022107733,0.01600053],"genre_scores_gemma":[0.8780218,0.00007760086,0.027260102,0.00020586188,0.00004437371,0.0003985431,0.08694309,0.0005962063,0.006452395],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99946207,0.000045493358,0.000022792661,0.00016472337,0.00020676927,0.00009821722],"domain_scores_gemma":[0.998852,0.00009204048,0.00020382425,0.00022984581,0.0003751756,0.0002470987],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00068797346,0.00036287226,0.00027352863,0.0013464502,0.00050559966,0.0004941885,0.0005378,0.00020385024,0.0035541402],"category_scores_gemma":[0.0012754926,0.0001478386,0.0003079212,0.00086292136,0.00021701967,0.00022942596,0.0010155273,0.00027403346,0.0022863455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006661841,0.0002811498,0.8487291,0.00010329379,0.000082100174,0.00027271785,0.00044780076,0.004361532,0.03275392,0.0029822695,0.024641639,0.08467834],"study_design_scores_gemma":[0.00008845437,0.00023875825,0.88274467,0.000021785665,0.00006333805,0.00043332067,0.00028840805,0.034422264,0.033075713,0.001111036,0.047480363,0.000031737098],"about_ca_topic_score_codex":0.008442616,"about_ca_topic_score_gemma":0.015457063,"teacher_disagreement_score":0.008442616,"about_ca_system_score_codex":0.0006539072,"about_ca_system_score_gemma":0.00042913546,"threshold_uncertainty_score":0.016786933},"labels":[],"label_agreement":null},{"id":"W4311131508","doi":"10.3847/1538-4357/ac9d3c","title":"VERTICO. IV. Environmental Effects on the Gas Distribution and Star Formation Efficiency of Virgo Cluster Spirals","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Victoria; Royal Military College of Canada; McMaster University; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; National Research Council Canada; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; Division of Astronomical Sciences; National Astronomical Observatory of Japan; National Radio Astronomy Observatory; Australian Research Council; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; California Institute of Technology; Gordon and Betty Moore Foundation; James S. McDonnell Foundation; National Science Foundation","keywords":"Physics; Virgo Cluster; Astrophysics; Cluster (spacecraft); Star cluster; Star formation; Astronomy; Star (game theory); Stars; Galaxy cluster; Galaxy","score_opus":0.005641635255794679,"score_gpt":0.190011880315248,"score_spread":0.18437024505945332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311131508","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9918122,0.00010262704,0.00028608445,0.000024352034,0.0000057292596,0.0000051641655,0.0008932878,0.000059374965,0.006811166],"genre_scores_gemma":[0.99660695,0.00005428294,0.0004888755,0.000008194927,0.000005882327,0.0000054872103,0.0015443537,0.000034171237,0.0012516843],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991643,0.000015083094,0.0000022736174,0.000029403847,0.000018270815,0.000018558892],"domain_scores_gemma":[0.99986136,0.000030440522,0.00003438928,0.000025697078,0.000019805644,0.000028202754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009806536,0.00013565266,0.00010892661,0.00039333553,0.00009269704,0.00050057535,0.00010488578,0.00010096199,0.0016441834],"category_scores_gemma":[0.00048493964,0.00006533068,0.000095937045,0.00045554645,0.000118689575,0.00010931182,0.00022393226,0.00009564903,0.0003438334],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065658096,0.00009083091,0.8753187,0.0000637588,0.00010584488,0.00075649016,0.0003363941,0.03123016,0.039021496,0.0026414515,0.003795763,0.04598249],"study_design_scores_gemma":[0.000013239013,0.000049235176,0.9747424,0.000014012941,0.000016509028,0.00010611507,0.00009276668,0.016412495,0.0026550991,0.0003106641,0.0055783186,0.000009095042],"about_ca_topic_score_codex":0.009615362,"about_ca_topic_score_gemma":0.014023689,"teacher_disagreement_score":0.009615362,"about_ca_system_score_codex":0.0002894618,"about_ca_system_score_gemma":0.000057973724,"threshold_uncertainty_score":0.019118786},"labels":[],"label_agreement":null},{"id":"W4311151793","doi":"10.3847/1538-4357/ac8ea8","title":"A Scintillation Arc Survey of 22 Pulsars with Low to Moderate Dispersion Measures","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":37,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia; Herzberg Institute of Astrophysics","funders":"Astrophysics Science Division; Division of Astronomical Sciences; Division of Physics; Nuclear Safety and Security Commission; National Science Foundation; University of Central Florida; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; National Radio Astronomy Observatory","keywords":"Pulsar; Physics; Scintillation; Astrophysics; Interstellar medium; Scattering; Spectral line; Line-of-sight; Anisotropy; Astronomy; Galaxy; Optics","score_opus":0.017051184894187277,"score_gpt":0.29635514103757227,"score_spread":0.279303956143385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311151793","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99929833,0.00003518551,0.0001785728,0.0000054830357,4.6591447e-7,0.0000034726884,0.00022205926,0.000011013071,0.00024537538],"genre_scores_gemma":[0.99879396,0.00004330392,0.00034123595,0.0000052520486,0.000004534593,0.000006450207,0.0006516637,0.000004435336,0.00014919997],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979573,0.00003378201,0.000017963644,0.000057065863,0.000047027446,0.000048410897],"domain_scores_gemma":[0.9991316,0.00014570102,0.00028475255,0.000108258144,0.00015826816,0.00017142562],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028673132,0.0001962399,0.00024266349,0.0014324997,0.0003820101,0.0003845913,0.00017502131,0.00013601936,0.00056423247],"category_scores_gemma":[0.00082834275,0.00013862622,0.00010896204,0.001225358,0.00018298914,0.00018809868,0.0006154123,0.00015459994,0.0002347192],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006781019,0.000023945622,0.98306364,0.0000112766775,0.000032173564,0.00009250999,0.00030625242,0.00015713504,0.00810669,0.000053413172,0.00016915349,0.007916018],"study_design_scores_gemma":[0.0000027426722,0.00005009394,0.9984971,0.000001576947,0.000011112326,0.00014630432,0.00009676896,0.00021542681,0.00042445064,0.000015300651,0.00053667405,0.0000023933583],"about_ca_topic_score_codex":0.0031711524,"about_ca_topic_score_gemma":0.0050986544,"teacher_disagreement_score":0.0031711524,"about_ca_system_score_codex":0.00019182506,"about_ca_system_score_gemma":0.0002129978,"threshold_uncertainty_score":0.0063053966},"labels":[],"label_agreement":null},{"id":"W4311160605","doi":"10.3847/1538-4357/ac9b58","title":"Discovery of a Filamentary Synchrotron Structure Connected to the Coherent Magnetic Field in the Outer Galaxy","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Brandon University; University of Calgary; University of Manitoba; National Research Council Canada; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Astrophysics Division; National Research Council Canada; Canadian Space Agency; Goddard Space Flight Center; University of Toronto; National Aeronautics and Space Administration; Canada Research Chairs; California Institute of Technology; Natural Sciences and Engineering Research Council of Canada; University of Hertfordshire; National Science Foundation","keywords":"Physics; Superbubble; Astrophysics; Supernova remnant; Galactic plane; Supernova; Pulsar; Galaxy; Astronomy; Nebula; Magnetic field; Interstellar medium; Bow shock (aerodynamics); Star formation; Stars; Shock wave","score_opus":0.005016050125671987,"score_gpt":0.2064698695790534,"score_spread":0.2014538194533814,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311160605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998733,0.000039440925,0.00023192084,0.000020087688,0.0000012027283,0.0000022544705,0.00009503763,0.000020433446,0.000856584],"genre_scores_gemma":[0.9992944,0.000015582547,0.00031321554,0.000017866058,0.0000054480347,0.0000021329804,0.00020295341,0.000004007276,0.00014442878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999354,0.0000053306153,0.0000030584886,0.000020251391,0.00001528696,0.000020609754],"domain_scores_gemma":[0.99960047,0.00004463545,0.00019288078,0.000043941764,0.000036687103,0.00008132197],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010053946,0.00013024526,0.00012329179,0.0007213472,0.00027960652,0.00051710365,0.00022876785,0.00021184556,0.00086771266],"category_scores_gemma":[0.0002662884,0.000158658,0.00011620222,0.00042097652,0.00032058515,0.00014374673,0.00033511076,0.00021757802,0.00016710674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024695348,0.000056525485,0.8223063,0.000026044892,0.000077808945,0.0010463257,0.00047123016,0.0002603753,0.16699712,0.00038733956,0.00045974954,0.0076642283],"study_design_scores_gemma":[0.0000070610276,0.000047801303,0.9945486,0.000004857118,0.000022815504,0.00042022867,0.0000796186,0.00034596288,0.0036251396,0.00007286035,0.00082172645,0.0000032149237],"about_ca_topic_score_codex":0.0025553934,"about_ca_topic_score_gemma":0.0032515856,"teacher_disagreement_score":0.0025553934,"about_ca_system_score_codex":0.00022782423,"about_ca_system_score_gemma":0.00007682089,"threshold_uncertainty_score":0.005080998},"labels":[],"label_agreement":null},{"id":"W4311178807","doi":"10.3847/1538-4357/ac982e","title":"The Relation between Globular Cluster Systems and Supermassive Black Holes in Spiral Galaxies. III. The Link to the M <sub>•</sub>–M <sub>*</sub> Correlation","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Consejo Nacional de Ciencia y Tecnología","keywords":"Physics; Astrophysics; Globular cluster; Galaxy; Supermassive black hole; Spiral galaxy; Stellar mass; Milky Way; Dwarf galaxy; Astronomy; Star formation","score_opus":0.007160538662037276,"score_gpt":0.19835834980822364,"score_spread":0.19119781114618636,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311178807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99764246,0.00034653724,0.00014345704,0.00025319486,0.0000053965728,0.0000027635958,0.00014405244,0.000008655956,0.0014533964],"genre_scores_gemma":[0.99965274,0.000040596333,0.000034442983,0.000018478968,0.000010835526,9.98411e-7,0.00006757134,0.0000017009479,0.0001727225],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997365,0.00007252914,0.000017505829,0.000047739595,0.00004780912,0.00007792357],"domain_scores_gemma":[0.9944794,0.0019514384,0.0020705496,0.00036525165,0.000377463,0.000755895],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000646455,0.00019023022,0.00018510497,0.0013652946,0.0003586848,0.00092773227,0.00034782945,0.0005409595,0.0062228255],"category_scores_gemma":[0.0045898487,0.0001704037,0.00028647148,0.0010675819,0.0008831443,0.00049307593,0.00071095553,0.00043143242,0.0005905553],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004823601,0.0000079012425,0.9978364,0.000004510759,0.000022970638,0.000036212165,0.000044988526,0.00010220117,0.00029201663,0.00023887338,0.00014130083,0.0012243084],"study_design_scores_gemma":[0.0000052173077,0.000018323899,0.9985662,0.000004954887,0.000020553249,0.00011026713,0.00012665261,0.00038427446,0.00009834401,0.00050388445,0.000158452,0.0000029015382],"about_ca_topic_score_codex":0.006134146,"about_ca_topic_score_gemma":0.007227835,"teacher_disagreement_score":0.0062228255,"about_ca_system_score_codex":0.00028358365,"about_ca_system_score_gemma":0.00024147765,"threshold_uncertainty_score":0.020817399},"labels":[],"label_agreement":null},{"id":"W4311244859","doi":"10.3847/1538-4357/ac9e01","title":"The Poor Old Heart of the Milky Way","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Australian Astronomical Optics-Macquarie; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; National Development and Reform Commission; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Harvard University; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Milky Way; Galaxy; Astrophysics; Stars; Population; Astrometry; Giant star; Astronomy; Medicine","score_opus":0.009124757800408334,"score_gpt":0.21360802196191794,"score_spread":0.2044832641615096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311244859","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966884,0.0001266373,0.00025179962,0.00008330899,0.0000041138155,0.000002941512,0.0006280381,0.000019981346,0.002194801],"genre_scores_gemma":[0.99618995,0.0001340314,0.000402776,0.00008086802,0.000007716777,0.0000042641464,0.001054686,0.000019820205,0.002105903],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998642,0.00001723173,0.0000063717353,0.000047921232,0.000030190182,0.000034159166],"domain_scores_gemma":[0.99972576,0.000032333253,0.00008601718,0.000037290665,0.000039495346,0.00007914108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013181742,0.00015356328,0.00034244196,0.00086124206,0.00046933003,0.001204785,0.00024421464,0.00025281674,0.0036370046],"category_scores_gemma":[0.00072560675,0.00009408558,0.00016380141,0.0010288561,0.00042907,0.0006192824,0.0010946018,0.00021669484,0.0008036918],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010508965,0.00002316795,0.9666341,0.000056802826,0.00007612513,0.00062559405,0.0021303818,0.0006864931,0.0032067685,0.0027154281,0.0033032296,0.020436844],"study_design_scores_gemma":[0.000010693147,0.000052297622,0.9707745,0.000029447898,0.000039947023,0.0006233216,0.0020436759,0.00083076826,0.00070465513,0.001991418,0.022886999,0.00001215842],"about_ca_topic_score_codex":0.0054292525,"about_ca_topic_score_gemma":0.009529854,"teacher_disagreement_score":0.0054292525,"about_ca_system_score_codex":0.00029511916,"about_ca_system_score_gemma":0.00024999623,"threshold_uncertainty_score":0.0121670365},"labels":[],"label_agreement":null},{"id":"W4311317986","doi":"10.3847/1538-4357/ac9e9f","title":"LoTSS Jellyfish Galaxies. IV. Enhanced Star Formation on the Leading Half of Cluster Galaxies and Gas Compression in IC3949","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; National Institutes of Natural Sciences; Max-Planck-Institut für Astrophysik; National Science and Technology Council; York University; Ministry of Science and Technology, Taiwan; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; U.S. Department of Energy; Smithsonian Institution; National Radio Astronomy Observatory; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Academia Sinica","keywords":"Physics; Jellyfish; Astrophysics; Astronomy; Galaxy; Luminous infrared galaxy; Galaxy cluster; Elliptical galaxy; Fishery","score_opus":0.009834059125555688,"score_gpt":0.21500522442819905,"score_spread":0.20517116530264337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311317986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993905,0.000030196174,0.00004114237,0.000005715477,4.5216876e-7,0.000001376617,0.00009328,0.000009394282,0.00042795847],"genre_scores_gemma":[0.9997458,0.000008192703,0.000039193226,0.0000027211508,7.6884135e-7,6.273472e-7,0.00009820988,0.0000012271107,0.00010338267],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999523,0.0000018113649,0.000002393557,0.000018511319,0.000008700009,0.000016243932],"domain_scores_gemma":[0.99974006,0.000016694428,0.00009915701,0.000029405053,0.000019994797,0.00009463063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005448802,0.00016510543,0.00015657097,0.00087304605,0.0003345649,0.00033406322,0.00024048897,0.00017295819,0.0018392132],"category_scores_gemma":[0.00019710457,0.000096284035,0.00025086608,0.00034827972,0.0002571508,0.00017326951,0.0004099847,0.00013160567,0.0002520711],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011883553,0.000017772447,0.9533365,0.00001463057,0.000026734362,0.00020706774,0.00027718954,0.0003607799,0.041045412,0.00014585705,0.00015615184,0.0042931363],"study_design_scores_gemma":[0.0000011439387,0.000011808811,0.99896,9.2154687e-7,0.0000027886833,0.00005131696,0.000056933295,0.00029042806,0.00050992594,0.000020622429,0.000093015755,0.0000011440402],"about_ca_topic_score_codex":0.009668572,"about_ca_topic_score_gemma":0.011520311,"teacher_disagreement_score":0.009668572,"about_ca_system_score_codex":0.00034078816,"about_ca_system_score_gemma":0.00008424302,"threshold_uncertainty_score":0.019224584},"labels":[],"label_agreement":null},{"id":"W4311318000","doi":"10.3847/1538-4357/ac9ea0","title":"The Neutron Star Population in M28: A Joint Chandra/GBT Look at Pulsar Paradise","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Precursory Research for Embryonic Science and Technology; Agencia Estatal de Investigación; Smithsonian Astrophysical Observatory; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; European Commission; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; Ministerio de Ciencia e Innovación; European Research Council; Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Physics; Astrophysics; Millisecond pulsar; Neutron star; Pulsar; Astronomy; Luminosity; Population; X-ray binary; Orbital period; Globular cluster; RADIUS; X-ray pulsar; Pulsar planet; Green Bank Telescope; Binary pulsar; Galaxy; Stars","score_opus":0.014512824313336808,"score_gpt":0.22504498269192613,"score_spread":0.21053215837858932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311318000","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99927825,0.000039971826,0.00003348714,0.000026594924,0.0000010444247,0.0000018875006,0.00021203009,0.000003576481,0.0004031342],"genre_scores_gemma":[0.99854654,0.000051431995,0.00024692726,0.00001532191,0.000006266727,0.000002837909,0.00077317515,0.0000062788117,0.00035118122],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999193,0.000006857367,0.0000028764166,0.00002827422,0.000022626971,0.000020096344],"domain_scores_gemma":[0.99975425,0.000022568933,0.0000664055,0.00003175956,0.000036551926,0.00008848903],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016219003,0.00015585985,0.00021494656,0.001149438,0.00033084245,0.00036466983,0.00022280925,0.000102040794,0.0007748407],"category_scores_gemma":[0.00052357727,0.00008888153,0.0001416763,0.00061294116,0.00023738097,0.00028800283,0.00094224646,0.00019915141,0.00021079803],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014525291,0.000033803193,0.98034793,0.000016818734,0.000035067627,0.00032445078,0.0006185297,0.0002884198,0.009429324,0.0002458772,0.00067520153,0.00783923],"study_design_scores_gemma":[0.0000035195587,0.000022590715,0.9973959,0.0000035595385,0.0000056150097,0.00019976821,0.00025964348,0.0003239897,0.00037391335,0.000091098074,0.0013164694,0.000003879816],"about_ca_topic_score_codex":0.005683298,"about_ca_topic_score_gemma":0.012499519,"teacher_disagreement_score":0.005683298,"about_ca_system_score_codex":0.0002234952,"about_ca_system_score_gemma":0.00019133276,"threshold_uncertainty_score":0.011300445},"labels":[],"label_agreement":null},{"id":"W4311350776","doi":"10.3847/1538-4357/aca01d","title":"Grain Growth in the Dust Ring with a Crescent around the Very Low-mass Star ZZ Tau IRS with JVLA","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Japan Society for the Promotion of Science","keywords":"Physics; Astrophysics; Planetesimal; Stars; Spectral energy distribution; Grain growth; Radiative transfer; Planet; Circumbinary planet; Planetary system; Cosmic dust; Accretion (finance); Interstellar medium; Astronomy; Grain size","score_opus":0.007653520133448385,"score_gpt":0.20672546981201123,"score_spread":0.19907194967856284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311350776","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993486,0.000023056298,0.00017389265,0.000008827173,0.0000013743189,0.0000015699122,0.0000957193,0.000019506308,0.00032742726],"genre_scores_gemma":[0.99947625,0.000005361647,0.00023945038,0.000005336904,0.0000022598867,0.0000015989397,0.00012749257,0.000005294231,0.0001369307],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999435,0.000005019088,0.000002838028,0.00001987649,0.000011381185,0.000017428922],"domain_scores_gemma":[0.99945086,0.00010275934,0.00016295501,0.000058391473,0.00010155577,0.00012350964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012101315,0.00010724163,0.00014903433,0.0004897943,0.0002452205,0.00043754667,0.00020546699,0.00016460211,0.0008098261],"category_scores_gemma":[0.00032121874,0.00011422025,0.00013604645,0.0002447879,0.00017967816,0.00017128108,0.00028325262,0.00014352691,0.00019981885],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093589624,0.00010796757,0.4729396,0.0000305576,0.000061308165,0.0007348579,0.00034462157,0.0026151014,0.51287955,0.00023496318,0.0004752064,0.00864029],"study_design_scores_gemma":[0.000012727349,0.000071688526,0.97711617,0.0000018372032,0.000011419084,0.00013881076,0.00013664631,0.0043712854,0.017762331,0.000042497344,0.00032853484,0.000006093629],"about_ca_topic_score_codex":0.002575532,"about_ca_topic_score_gemma":0.0029073737,"teacher_disagreement_score":0.002575532,"about_ca_system_score_codex":0.00035475442,"about_ca_system_score_gemma":0.000068086425,"threshold_uncertainty_score":0.0051210523},"labels":[],"label_agreement":null},{"id":"W4311465523","doi":"10.3847/1538-4357/ac9dee","title":"Resolved Molecular Gas Observations of MaNGA Post-starbursts Reveal a Tumultuous Past","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of Waterloo","funders":"Lawrence Berkeley National Laboratory; Hsinchu Science Park Bureau, Ministry of Science and Technology, Taiwan; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; National Institutes of Natural Sciences; Max-Planck-Institut für Astrophysik; National Science and Technology Council; Fundação de Amparo à Pesquisa do Estado do Rio Grande do Sul; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; U.S. Department of Energy; Smithsonian Institution; National Radio Astronomy Observatory; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; Danmarks Grundforskningsfond; Leibniz-Gemeinschaft; University of Notre Dame; Ohio State University; National Research Foundation; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; National Science Foundation; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Academia Sinica","keywords":"Physics; Astrophysics; Galaxy; Star formation; Astronomy; Galaxy merger; Luminous infrared galaxy; Galaxy formation and evolution","score_opus":0.010526354781099466,"score_gpt":0.21022566954538072,"score_spread":0.19969931476428124,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311465523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992036,0.000055229793,0.000036638452,0.000019245157,0.0000012350628,0.0000013694831,0.00017494138,0.0000074653644,0.00050045573],"genre_scores_gemma":[0.9995703,0.000018187578,0.000057907037,0.0000074218256,0.0000031618442,0.0000010880207,0.00018434839,0.0000019134768,0.00015557914],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999944,0.000004045156,0.0000021613248,0.000016551812,0.000009321492,0.000024004601],"domain_scores_gemma":[0.9996387,0.000023992328,0.00013548022,0.000025230938,0.000039716484,0.00013686312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108901695,0.00010630138,0.00013596009,0.00065181276,0.00040799548,0.0004794023,0.00018260776,0.00016763885,0.0013905772],"category_scores_gemma":[0.00022784271,0.000109206376,0.000096366704,0.00045072378,0.00025730947,0.000201713,0.00024302516,0.00020763231,0.00027141767],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000089917456,0.000039798397,0.96259487,0.0000110615065,0.000017484803,0.00012511024,0.00023934213,0.0001027009,0.033644415,0.00015042837,0.00015955426,0.0028252918],"study_design_scores_gemma":[7.638474e-7,0.000009697202,0.9994855,9.234484e-7,0.0000021097303,0.000024790505,0.000052175586,0.000076920216,0.00022573229,0.000013990575,0.00010671221,5.43377e-7],"about_ca_topic_score_codex":0.0081027355,"about_ca_topic_score_gemma":0.01494392,"teacher_disagreement_score":0.0081027355,"about_ca_system_score_codex":0.00032386722,"about_ca_system_score_gemma":0.00011086112,"threshold_uncertainty_score":0.016111135},"labels":[],"label_agreement":null},{"id":"W4311465525","doi":"10.3847/1538-4357/ac9f18","title":"Is the Hot, Dense Sub-Neptune TOI-824 b an Exposed Neptune Mantle? Spitzer Detection of the Hot Dayside and Reanalysis of the Interior Composition","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Université du Québec","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada","keywords":"Neptune; Physics; Astrobiology; Mantle (geology); Astronomy; Astrophysics; Planet; Geophysics","score_opus":0.00863592108663601,"score_gpt":0.20119062836493176,"score_spread":0.19255470727829574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311465525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950794,0.00020931893,0.0004481635,0.0000874714,0.000009121737,0.0000042852444,0.00040882372,0.000061314575,0.0036921732],"genre_scores_gemma":[0.9981877,0.00012916396,0.0004708963,0.00004683808,0.000014112219,0.0000031817983,0.0005072063,0.000021625396,0.00061907485],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996674,0.0000016580287,0.0000013274251,0.000011753075,0.000009086258,0.00000948958],"domain_scores_gemma":[0.99993336,0.000005958345,0.00002084802,0.000008041285,0.000009952595,0.000021922757],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000060169106,0.00014979554,0.00014517337,0.00041848698,0.00027306456,0.000383811,0.0002105401,0.00021183507,0.0020275097],"category_scores_gemma":[0.00015418172,0.00009886835,0.00009833786,0.00027383392,0.00022842758,0.00022041271,0.00027079394,0.00018500582,0.0005835162],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044503398,0.000036852784,0.42283428,0.0000697764,0.00006295926,0.00087257405,0.000558376,0.00032740945,0.5534528,0.00039897382,0.0012204372,0.0197205],"study_design_scores_gemma":[0.000007813263,0.0000319953,0.98238313,0.000009163687,0.00002059972,0.0005437292,0.0003235401,0.000747581,0.011277663,0.000212303,0.0044359094,0.0000065805],"about_ca_topic_score_codex":0.002856738,"about_ca_topic_score_gemma":0.0034517073,"teacher_disagreement_score":0.002856738,"about_ca_system_score_codex":0.00019252043,"about_ca_system_score_gemma":0.0000507176,"threshold_uncertainty_score":0.0067827106},"labels":[],"label_agreement":null},{"id":"W4311487980","doi":"10.3847/1538-4357/ac8b78","title":"Follow-up of Young Stars Identified with BANYAN Σ: New Low-mass Members of Nearby Moving Groups","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; University of California, Los Angeles; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Space Telescope Science Institute; Johns Hopkins University; Queen's University Belfast; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Central University; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; Smithsonian Institution; Durham University; Rice University","keywords":"Physics; Stars; Banyan; Astrophysics; Accretion (finance); Population; Astronomy; Medicine","score_opus":0.008689053107571698,"score_gpt":0.20747328701996418,"score_spread":0.19878423391239247,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311487980","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999572,0.00003536458,0.00008863336,0.0000057812194,0.0000013993085,0.0000044731014,0.000038775444,0.0000030738192,0.00025046137],"genre_scores_gemma":[0.9995783,0.000020691117,0.00010096744,0.00000723813,0.0000031052205,0.0000028125335,0.00010130076,0.0000013118885,0.0001843112],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978024,0.00003489547,0.000018584027,0.00006251114,0.00005030845,0.00005343288],"domain_scores_gemma":[0.9990181,0.00016228626,0.00029929448,0.000099863304,0.00017412133,0.00024640947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003785583,0.0001468376,0.00021105162,0.0013496482,0.0005797838,0.00035241476,0.00027607393,0.00024695063,0.00091510185],"category_scores_gemma":[0.0011926049,0.00010057733,0.0001439776,0.00046226726,0.00019252318,0.00032396728,0.0005064937,0.00026082402,0.0003008681],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000043655593,0.000021352587,0.99410546,0.000003304986,0.0000060187144,0.00021568744,0.00022227237,0.000012299085,0.003021035,0.000010937739,0.000028810427,0.002309053],"study_design_scores_gemma":[0.0000012112824,0.00007571342,0.9980373,0.0000017931272,0.000007778174,0.00045678893,0.0002584377,0.00007596019,0.00090443436,0.000013822617,0.00016518055,0.0000017860427],"about_ca_topic_score_codex":0.003537256,"about_ca_topic_score_gemma":0.0052054278,"teacher_disagreement_score":0.003537256,"about_ca_system_score_codex":0.00015262346,"about_ca_system_score_gemma":0.00013099606,"threshold_uncertainty_score":0.007033348},"labels":[],"label_agreement":null},{"id":"W4311488578","doi":"10.3847/1538-4357/ac9c07","title":"The Obscured Fraction of Quasars at Cosmic Noon","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Redshift; Luminosity; Active galactic nucleus; Galaxy","score_opus":0.007821667798040943,"score_gpt":0.21370909972865185,"score_spread":0.2058874319306109,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311488578","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977059,0.000113611706,0.00022962193,0.000017978382,0.0000032032376,0.0000029526666,0.00064728723,0.000021896232,0.0012576065],"genre_scores_gemma":[0.9987214,0.00003797481,0.0000680147,0.000008728377,0.000009510431,0.0000016391331,0.0007664625,0.000004121209,0.00038201193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999595,0.000056138535,0.000023707116,0.00009519961,0.00012954223,0.00010050251],"domain_scores_gemma":[0.99706846,0.0005073512,0.0011400379,0.00040710438,0.0003146033,0.0005625112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042274396,0.0002284228,0.00018164833,0.0019918876,0.00021589076,0.0008001987,0.00035192643,0.00022048924,0.0028231551],"category_scores_gemma":[0.0025332598,0.00014129988,0.00021726543,0.0006910955,0.00029885775,0.00039923022,0.00043789943,0.00016853155,0.000530981],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006430805,0.0000125176375,0.99258536,0.000007285364,0.000040152743,0.00011377354,0.00007153967,0.00039042672,0.0030072385,0.0002300273,0.00021296844,0.0032642675],"study_design_scores_gemma":[7.8776685e-7,0.000013708842,0.9987136,0.0000016413086,0.0000071321037,0.00014824243,0.000026634478,0.00046262803,0.00028810182,0.00004855944,0.00028710588,0.0000018226337],"about_ca_topic_score_codex":0.0030245634,"about_ca_topic_score_gemma":0.0028222948,"teacher_disagreement_score":0.0030245634,"about_ca_system_score_codex":0.00023915818,"about_ca_system_score_gemma":0.000088435474,"threshold_uncertainty_score":0.009444356},"labels":[],"label_agreement":null},{"id":"W4311533642","doi":"10.3847/1538-4357/ac9cd2","title":"Measuring the Ellipticity of M87* Images","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"National Science Foundation","keywords":"Physics; Supermassive black hole; Galaxy; Astrophysics; Measure (data warehouse); Black hole (networking); Shadow (psychology); Event horizon; Event (particle physics)","score_opus":0.021471729189884575,"score_gpt":0.22276067096653215,"score_spread":0.20128894177664758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311533642","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99364036,0.00008259679,0.0036648645,0.000047176683,0.000006741408,0.000011895202,0.000649009,0.00017778775,0.0017195],"genre_scores_gemma":[0.99629104,0.000029841814,0.00250457,0.000015901674,0.0000053464355,0.0000051580796,0.0010152165,0.000042707677,0.0000902403],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971324,0.000056444638,0.000015560528,0.00007415349,0.00008819677,0.000052345935],"domain_scores_gemma":[0.9990608,0.00024545586,0.00022366768,0.00021256658,0.00016416477,0.00009343136],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007969638,0.00028403848,0.0002390246,0.0007770268,0.00020199611,0.00072261837,0.0002573892,0.00025320562,0.0008806658],"category_scores_gemma":[0.0019299907,0.00023957764,0.00036864536,0.00053635257,0.0004042645,0.00023609822,0.00045376518,0.00028746872,0.00022330947],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010919705,0.00018852997,0.3864618,0.00022990038,0.00055892306,0.0004900726,0.00047235654,0.27416214,0.29100198,0.0068367696,0.0027045878,0.035800952],"study_design_scores_gemma":[0.000060969975,0.00020479129,0.4831935,0.000035229183,0.00010194427,0.0005526676,0.00019290336,0.4084569,0.1020176,0.0020048618,0.0031208443,0.000057837682],"about_ca_topic_score_codex":0.0012092411,"about_ca_topic_score_gemma":0.0008500719,"teacher_disagreement_score":0.0012092411,"about_ca_system_score_codex":0.00049141754,"about_ca_system_score_gemma":0.00011367199,"threshold_uncertainty_score":0.0042147636},"labels":[],"label_agreement":null},{"id":"W4311533707","doi":"10.3847/1538-4357/aca08b","title":"The Cavity of 3CR 196.1: Hα Emission Spatially Associated with an X-Ray Cavity","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministero dell’Istruzione, dell’Università e della Ricerca; National Aeronautics and Space Administration; Agencia Nacional de Investigación y Desarrollo; Dipartimenti di Eccellenza; Smithsonian Institution","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Astronomy; Galaxy cluster; Radio galaxy; Cluster (spacecraft); Telescope; Brightest cluster galaxy; Cavity wall; Geology","score_opus":0.006681574972533151,"score_gpt":0.20722318630538505,"score_spread":0.2005416113328519,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311533707","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990934,0.00006500262,0.00010803525,0.0000069433927,0.000001353242,0.0000030847812,0.0001309851,0.00002233807,0.00056881004],"genre_scores_gemma":[0.9993892,0.000020563753,0.00017758665,0.0000055467654,0.0000029337532,0.0000017200259,0.00020231037,0.000005006652,0.00019503891],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999949,0.0000021087933,0.0000013639033,0.000016736101,0.000010682366,0.000020166557],"domain_scores_gemma":[0.99985874,0.00000973037,0.00006441095,0.0000112952985,0.000011811784,0.000044063414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004376954,0.00023397693,0.00020163877,0.0008092923,0.00025779175,0.00037571447,0.00025989264,0.0001923995,0.0013941614],"category_scores_gemma":[0.000093490584,0.00011720891,0.00023413404,0.00047481625,0.00024210493,0.00010672888,0.00033205774,0.00015862094,0.00036319724],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009920718,0.00011055727,0.37745723,0.00008314667,0.00006909522,0.0031901312,0.00047725742,0.00062396174,0.60608476,0.00028369756,0.0004588331,0.010169168],"study_design_scores_gemma":[0.000012788493,0.000059838996,0.993341,0.0000045254665,0.000015505455,0.00079147075,0.000114142174,0.0004264872,0.00464853,0.00003947681,0.0005420021,0.0000041912203],"about_ca_topic_score_codex":0.003994934,"about_ca_topic_score_gemma":0.0031459285,"teacher_disagreement_score":0.003994934,"about_ca_system_score_codex":0.00022551887,"about_ca_system_score_gemma":0.00007854522,"threshold_uncertainty_score":0.007943392},"labels":[],"label_agreement":null},{"id":"W4311787584","doi":"10.3847/1538-4357/ac9eae","title":"Electron Density Variations in the Interstellar Medium and the Average Frequency Profile of a Scintle from Pulsar Scintillation Spectra","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; York University","funders":"Russian Academy of Sciences; Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Wavenumber; Pulsar; Spectral line; Astrophysics; Scintillation; Scattering; Interstellar medium; Spectral density; Computational physics; Context (archaeology); Optics; Astronomy; Statistics; Galaxy","score_opus":0.004421146639776736,"score_gpt":0.20630751255009191,"score_spread":0.20188636591031517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311787584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99887484,0.000040423205,0.0006223053,0.000004080921,0.0000011666662,9.980262e-7,0.0000726326,0.000015473077,0.00036809748],"genre_scores_gemma":[0.9997198,0.000016253682,0.00014294397,6.339538e-7,0.0000013255163,5.334233e-7,0.00007697979,0.0000023072373,0.00003924356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996066,0.0000056278277,0.0000024582503,0.000008668552,0.000015392663,0.0000071219933],"domain_scores_gemma":[0.9996325,0.00014706707,0.000088517336,0.000026625543,0.00007291585,0.00003228624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014819851,0.00011751947,0.0001138892,0.0012744343,0.00014126473,0.00028373778,0.000113055714,0.000103946455,0.00073874317],"category_scores_gemma":[0.000789521,0.000081582,0.000085809865,0.00049612555,0.00017909199,0.00017789859,0.00019529929,0.000101844045,0.00010803906],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003017294,0.00003868303,0.6319607,0.000059328715,0.00005980521,0.00046912895,0.00040207608,0.005822133,0.3284625,0.0008198364,0.00017347246,0.03143063],"study_design_scores_gemma":[0.000003754823,0.000067017405,0.97524375,0.000006125236,0.000015432315,0.00044283617,0.00009406683,0.009495795,0.014056323,0.00023462353,0.00032685156,0.000013450154],"about_ca_topic_score_codex":0.0009202995,"about_ca_topic_score_gemma":0.0012619921,"teacher_disagreement_score":0.0012744343,"about_ca_system_score_codex":0.00011423867,"about_ca_system_score_gemma":0.000055889454,"threshold_uncertainty_score":0.0024713278},"labels":[],"label_agreement":null},{"id":"W4311881196","doi":"10.3847/1538-4357/aca1c5","title":"Central Star Formation in Early-type Galaxy I Zw 81 in the Bootes Void","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Surface brightness; Lenticular galaxy; Interacting galaxy; Elliptical galaxy; Star formation","score_opus":0.008054194782446431,"score_gpt":0.2056211224364691,"score_spread":0.19756692765402267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311881196","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998073,0.000011498214,0.000015038949,0.0000028889212,2.1548831e-7,6.6229575e-7,0.000021300604,0.0000014532477,0.00013966009],"genre_scores_gemma":[0.99982077,0.000008456643,0.000023513223,0.0000013367152,5.041591e-7,4.460013e-7,0.00005342368,5.354053e-7,0.00009102558],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999573,0.0000031543327,0.0000021032956,0.000010659334,0.000007633548,0.000019085533],"domain_scores_gemma":[0.999869,0.000010984714,0.000047696543,0.000008923835,0.000010980158,0.00005245014],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007698127,0.00013494489,0.00015849152,0.0005887232,0.00029279722,0.00037225673,0.00013878109,0.00015459862,0.0007467182],"category_scores_gemma":[0.00016663133,0.000078099554,0.000088949026,0.00031606245,0.00030187258,0.00017475733,0.0004807557,0.000094705865,0.00008956499],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015626733,0.00005852708,0.9718382,0.000013700897,0.000021842,0.0017022991,0.00065973453,0.00051835825,0.020240525,0.00029390323,0.00010489151,0.004391849],"study_design_scores_gemma":[0.0000030940648,0.000037830778,0.9977518,0.00000241532,0.0000048230695,0.0002811657,0.00045132815,0.00044217886,0.0007326718,0.00006732043,0.00022329901,0.0000020736725],"about_ca_topic_score_codex":0.014793078,"about_ca_topic_score_gemma":0.021584654,"teacher_disagreement_score":0.014793078,"about_ca_system_score_codex":0.00041179784,"about_ca_system_score_gemma":0.00015162492,"threshold_uncertainty_score":0.029413939},"labels":[],"label_agreement":null},{"id":"W4311891261","doi":"10.3847/1538-4357/ac9cdc","title":"Herschel Optimized Tau and Temperature (HOTT) Maps: Uncertainty Analysis and Robust Parameter Extraction","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Black-body radiation; Spectral energy distribution; Astrophysics; Noise (video); Optics","score_opus":0.009871150957615886,"score_gpt":0.23798646780342655,"score_spread":0.22811531684581066,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311891261","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1127366,0.0006190241,0.83980685,0.0004374469,0.00007898679,0.00015142854,0.019630076,0.020669078,0.0058705225],"genre_scores_gemma":[0.51324415,0.00025881708,0.46106294,0.00013794693,0.0001250138,0.0002449349,0.018701307,0.0044495948,0.0017752995],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99871373,0.000327693,0.00006759889,0.00026239172,0.0005008486,0.000127715],"domain_scores_gemma":[0.9957367,0.0017236382,0.00056170573,0.0012037967,0.00067812763,0.00009596648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0035830594,0.0011437922,0.0006221478,0.0028059047,0.000624434,0.0025576514,0.001214768,0.0006609153,0.005110126],"category_scores_gemma":[0.015492159,0.00057773315,0.0011905761,0.0018613907,0.0004947725,0.0016792981,0.0024053266,0.0012480667,0.0019977705],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041709526,0.00015427258,0.037171803,0.00044628038,0.0007461675,0.0005080391,0.0004562514,0.5584374,0.016573897,0.048720337,0.029261446,0.30710703],"study_design_scores_gemma":[0.000053394233,0.000056233675,0.024584843,0.00006891761,0.000075863834,0.00023238386,0.000105823376,0.8735548,0.022489736,0.050750773,0.027850635,0.00017659353],"about_ca_topic_score_codex":0.006307768,"about_ca_topic_score_gemma":0.0040124403,"teacher_disagreement_score":0.006307768,"about_ca_system_score_codex":0.00074357743,"about_ca_system_score_gemma":0.0009524781,"threshold_uncertainty_score":0.01894927},"labels":[],"label_agreement":null},{"id":"W4311943333","doi":"10.3847/1538-4357/ac9ea4","title":"Evaluating Lyα Emission as a Tracer of the Largest Cosmic Structure at z ∼ 2.47","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Saint Mary's University","funders":"Nuclear Safety and Security Commission; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; Compute Canada; Canadian Foundation for AIDS Research; Purdue University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; COSMIC cancer database; Context (archaeology); Astronomy; Active galactic nucleus; Population; Supercluster (genetic); Galaxy formation and evolution; Paleontology","score_opus":0.011187725178514744,"score_gpt":0.25498967140880774,"score_spread":0.243801946230293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4311943333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975224,0.00011037763,0.0006516512,0.000013217511,0.0000016136305,0.000004504204,0.00018366707,0.000033796096,0.0014786558],"genre_scores_gemma":[0.9992481,0.000038745547,0.0003307923,0.000008953839,0.0000032926046,0.0000027392045,0.00019620321,0.0000054167244,0.00016569131],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999291,0.0000056212134,0.0000028243896,0.000020894286,0.000015793057,0.00002581956],"domain_scores_gemma":[0.99960667,0.000042547457,0.00015315472,0.000025798783,0.000048381255,0.0001234654],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019642392,0.00018616948,0.000116597796,0.0012294485,0.00017910189,0.0006289821,0.00016505821,0.00018995455,0.0011696372],"category_scores_gemma":[0.0003400103,0.00011733572,0.00010790829,0.0005031046,0.00021051623,0.00030159295,0.00043662792,0.0001807954,0.00023858243],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016445722,0.000020191626,0.8532476,0.000021600565,0.000043512915,0.00030883128,0.0002242511,0.00027388832,0.13756767,0.00037633904,0.00020966926,0.007541999],"study_design_scores_gemma":[0.0000014316868,0.000027320624,0.99311465,0.0000024243438,0.000009118629,0.00014195635,0.00010845698,0.00039564725,0.0057843397,0.000060411414,0.00035217157,0.0000020639147],"about_ca_topic_score_codex":0.0014151279,"about_ca_topic_score_gemma":0.0026056266,"teacher_disagreement_score":0.0014151279,"about_ca_system_score_codex":0.00022508453,"about_ca_system_score_gemma":0.00005834004,"threshold_uncertainty_score":0.003912866},"labels":[],"label_agreement":null},{"id":"W4312037512","doi":"10.3847/1538-4357/aca409","title":"Tidal Distortions as a Bottleneck on Constraining Exoplanet Compositions","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Fonds de Recherche du Québec – Nature et Technologies","funders":"Fonds de recherche du Québec – Nature et technologies","keywords":"Exoplanet; Planet; RADIUS; Physics; Error bar; Transit (satellite); Astrophysics; Stellar density; Terrestrial planet; Amplitude; Tidal acceleration; Bottleneck; Astronomy; Stars","score_opus":0.012721154506754756,"score_gpt":0.23174486272077474,"score_spread":0.21902370821401998,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312037512","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9825646,0.0007617136,0.012744745,0.0002847665,0.000011257955,0.000010188325,0.00032549934,0.00013272738,0.0031645796],"genre_scores_gemma":[0.99819666,0.00008921591,0.0014521575,0.000015358111,0.0000051888946,0.0000021173917,0.00010749543,0.000019633846,0.000112065216],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99919623,0.00021207315,0.00007251476,0.0002246603,0.000236531,0.000057899997],"domain_scores_gemma":[0.99510527,0.0026338533,0.0010003016,0.000630599,0.00046396194,0.00016606173],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017658729,0.00036008094,0.0004210385,0.0012365557,0.00063908723,0.0015198425,0.00068663293,0.00028705134,0.0010716537],"category_scores_gemma":[0.0093908645,0.00032611072,0.00026084663,0.0011165922,0.000958542,0.0013616302,0.0014522853,0.0003860095,0.00023564529],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020935369,0.000018395358,0.92832845,0.00010369888,0.00011339436,0.00029546727,0.00078622834,0.016563633,0.018438594,0.0054958374,0.00048338537,0.029163508],"study_design_scores_gemma":[0.000021449165,0.00011517083,0.83948225,0.000086759756,0.00010014473,0.001102897,0.0012132851,0.11147841,0.022194054,0.016439134,0.00771278,0.000053654196],"about_ca_topic_score_codex":0.0042826044,"about_ca_topic_score_gemma":0.0053791995,"teacher_disagreement_score":0.0042826044,"about_ca_system_score_codex":0.00058700534,"about_ca_system_score_gemma":0.00026624932,"threshold_uncertainty_score":0.009338975},"labels":[],"label_agreement":null},{"id":"W4312037525","doi":"10.3847/1538-4357/aca27d","title":"The Star Formation Rate of the Milky Way as Seen by Herschel","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Horizon 2020 Framework Programme; Istituto Nazionale di Astrofisica","keywords":"Physics; Milky Way; Galactic plane; Astrophysics; Star formation; RADIUS; Galaxy; Computer science","score_opus":0.007484061699403787,"score_gpt":0.22220632990118477,"score_spread":0.21472226820178097,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312037525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9914568,0.0006368046,0.0010280265,0.00006431149,0.000005826047,0.000005417613,0.0015950213,0.00013100376,0.005076923],"genre_scores_gemma":[0.99739146,0.00012141706,0.00067191554,0.000009497656,0.0000054880848,0.000004664496,0.0011927526,0.000017732575,0.0005851008],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996685,0.00006023056,0.000014676056,0.00010864737,0.000104364255,0.000043656324],"domain_scores_gemma":[0.99888545,0.00025385825,0.00039233157,0.00020656033,0.00018784624,0.00007381914],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006260996,0.00012903947,0.00014284259,0.0011235735,0.000105487794,0.0007437649,0.00026954466,0.00019743637,0.0010521229],"category_scores_gemma":[0.002844665,0.0000971406,0.00030066134,0.0006298012,0.00020996357,0.00066934124,0.0004972298,0.00015656976,0.0004312441],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010530889,0.000014204191,0.9534631,0.00005374396,0.00012861165,0.00014087478,0.0005812685,0.0067987605,0.004680134,0.00330809,0.0016736276,0.02905227],"study_design_scores_gemma":[0.000007460978,0.00002601119,0.9786107,0.000018829232,0.000024227898,0.00020082465,0.000120343146,0.008504562,0.0021269438,0.00086508965,0.009476904,0.000017985356],"about_ca_topic_score_codex":0.0054489416,"about_ca_topic_score_gemma":0.004301011,"teacher_disagreement_score":0.0054489416,"about_ca_system_score_codex":0.00050436985,"about_ca_system_score_gemma":0.00011194636,"threshold_uncertainty_score":0.0108344555},"labels":[],"label_agreement":null},{"id":"W4312037587","doi":"10.3847/1538-4357/ac9d38","title":"Harvesting BAT-GUANO with NITRATES (Non-Imaging Transient Reconstruction and Temporal Search): Detecting and Localizing the Faintest Gamma-Ray Bursts with a Likelihood Framework","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Science Foundation","keywords":"Gamma-ray burst; Physics; Population; Astrophysics; Unavailability; Astronomy; Statistics","score_opus":0.007351516246678694,"score_gpt":0.20690957651849784,"score_spread":0.19955806027181916,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312037587","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.12565467,0.00020993914,0.8710127,0.00033441826,0.00001858136,0.0000365743,0.00014541963,0.00091167574,0.0016760539],"genre_scores_gemma":[0.7385308,0.00017687038,0.2578012,0.00015629805,0.000051980907,0.000074521944,0.00056136545,0.00026260407,0.0023843849],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997009,0.00009289443,0.000009559605,0.000065905384,0.000081126025,0.000049651113],"domain_scores_gemma":[0.99942446,0.00021988161,0.00012714768,0.0000806789,0.00007451574,0.000073469775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010704885,0.00047817413,0.00048101816,0.00039396202,0.0002541804,0.0008903013,0.0011940383,0.00061055453,0.0008459206],"category_scores_gemma":[0.002162749,0.00030405185,0.0006768536,0.00029544174,0.00082031614,0.0009198358,0.0013056918,0.0005521431,0.000273489],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007416456,0.0002113733,0.020044016,0.00020634968,0.00018368213,0.00047184143,0.00029294327,0.7050433,0.07949346,0.06815745,0.0021781428,0.12297582],"study_design_scores_gemma":[0.000005411266,0.000025427667,0.0008159132,0.0000043605537,0.0000052546065,0.000040363982,0.00001574496,0.9927037,0.0024170282,0.0036081234,0.00034971198,0.000008929816],"about_ca_topic_score_codex":0.0037029898,"about_ca_topic_score_gemma":0.004740979,"teacher_disagreement_score":0.0037029898,"about_ca_system_score_codex":0.0004988703,"about_ca_system_score_gemma":0.0008956421,"threshold_uncertainty_score":0.007362902},"labels":[],"label_agreement":null},{"id":"W4312070186","doi":"10.3847/1538-4357/ac9dfb","title":"The JCMT BISTRO-2 Survey: Magnetic Fields of the Massive DR21 Filament","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; McMaster University; Queen's University; University of Manitoba; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; Science and Engineering Research Board; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; Chinese Academy of Sciences; Department of Science and Technology, Ministry of Science and Technology, India; National Natural Science Foundation of China; Academia Sinica; Science and Technology Facilities Council; National Research Foundation","keywords":"Physics; James Clerk Maxwell Telescope; Protein filament; Magnetic field; Astrophysics; Polarization (electrochemistry); Star formation; Galaxy","score_opus":0.009763249742299121,"score_gpt":0.22322436053172978,"score_spread":0.21346111078943067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312070186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99518883,0.00011848639,0.00017624577,0.00005062101,0.0000035645226,0.00001012842,0.0020788664,0.000087102744,0.0022861601],"genre_scores_gemma":[0.9955617,0.00008620848,0.0004945301,0.00004347221,0.000027250406,0.000010669204,0.0033960724,0.000023330704,0.00035670603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998,0.000019420675,0.000010433037,0.00006481137,0.000057644706,0.00004756421],"domain_scores_gemma":[0.9993617,0.000044879755,0.00022988503,0.00010962438,0.000076379074,0.00017752875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020791599,0.00023520041,0.00023239927,0.0012691118,0.00035303566,0.0004908183,0.00033411672,0.0003302374,0.0013333795],"category_scores_gemma":[0.0004939639,0.0001456841,0.00020113721,0.0008064989,0.00016634002,0.00024857753,0.00070586184,0.00019894967,0.00047267848],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000325942,0.00008324987,0.897445,0.00008735476,0.00018813036,0.00069966336,0.00053400703,0.0009754519,0.08226439,0.00023110856,0.0023729098,0.014792781],"study_design_scores_gemma":[0.000007845188,0.000015909316,0.9967811,0.0000030506378,0.000013648743,0.00014125292,0.000040098064,0.00046176475,0.0010909887,0.0000139152335,0.0014262925,0.000004183669],"about_ca_topic_score_codex":0.0047644563,"about_ca_topic_score_gemma":0.0072130687,"teacher_disagreement_score":0.0047644563,"about_ca_system_score_codex":0.00036597255,"about_ca_system_score_gemma":0.00012819655,"threshold_uncertainty_score":0.009473443},"labels":[],"label_agreement":null},{"id":"W4312074043","doi":"10.3847/1538-4357/ac99e0","title":"The JCMT BISTRO Survey: A Spiral Magnetic Field in a Hub-filament Structure, Monoceros R2","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; McMaster University; Queen's University; University of Manitoba; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; Science and Engineering Research Board; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; Department of Science and Technology, Ministry of Science and Technology, India; National Natural Science Foundation of China; Academia Sinica; Science and Technology Facilities Council; National Research Foundation; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"James Clerk Maxwell Telescope; Physics; Magnetic field; Astrophysics; Magnetic pressure; Protein filament; Turbulence; Star formation; Magnetization; Galaxy; Mechanics; Chemistry","score_opus":0.011393121482426938,"score_gpt":0.23745216962661822,"score_spread":0.22605904814419128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312074043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983125,0.000054357744,0.000076048185,0.000020138008,0.0000016141602,0.000005277995,0.0005063721,0.000025781996,0.0009979382],"genre_scores_gemma":[0.9980082,0.000032133383,0.00032103778,0.00002140004,0.000008739545,0.00000636288,0.0012202209,0.000009256205,0.00037274646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984586,0.000013002054,0.00000712933,0.000043954646,0.000046690966,0.00004331861],"domain_scores_gemma":[0.9994729,0.000022953105,0.00021092313,0.00006510463,0.00006214324,0.00016597121],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019723656,0.0002163903,0.00019351997,0.0010570493,0.0004488379,0.0003176314,0.00031203905,0.00019442326,0.0007085331],"category_scores_gemma":[0.0003523961,0.00013467956,0.0001459999,0.0006109692,0.0002096469,0.00016666105,0.00049286406,0.0001249224,0.00021114865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038674442,0.00007083674,0.9416799,0.000039391103,0.00008246661,0.0008314746,0.00075653713,0.0005777698,0.04437975,0.00019574775,0.001319238,0.009680176],"study_design_scores_gemma":[0.000007952287,0.000020779406,0.99812335,0.0000023947496,0.0000061896876,0.00012279571,0.000083376115,0.00045236832,0.00043642652,0.000009704473,0.00073218177,0.0000023353164],"about_ca_topic_score_codex":0.021166928,"about_ca_topic_score_gemma":0.045805346,"teacher_disagreement_score":0.021166928,"about_ca_system_score_codex":0.00051091396,"about_ca_system_score_gemma":0.00023586825,"threshold_uncertainty_score":0.042087436},"labels":[],"label_agreement":null},{"id":"W4312186133","doi":"10.3847/1538-4357/ac9c66","title":"Creating the Radius Gap without Mass Loss","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"McGill University","keywords":"RADIUS; Physics; Population; Accretion (finance); Astrophysics; Algorithm; Computer science","score_opus":0.013113024507332992,"score_gpt":0.24581783519876568,"score_spread":0.2327048106914327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4312186133","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90935844,0.0014706366,0.054985315,0.0009658827,0.00016331727,0.000024233981,0.00020026354,0.0019452672,0.030886708],"genre_scores_gemma":[0.99685436,0.00006330157,0.0018336335,0.00008278259,0.000016183896,0.000007758204,0.000051715815,0.000082108854,0.0010081403],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998018,0.000038390383,0.00000865656,0.00006253103,0.000044584278,0.00004400522],"domain_scores_gemma":[0.9987814,0.00035114927,0.00030287317,0.00032224145,0.00009570092,0.00014666229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037541302,0.00033175776,0.0004014818,0.0003537278,0.0003192191,0.001011858,0.00079279364,0.000548912,0.0042932257],"category_scores_gemma":[0.003415461,0.00020398169,0.00026547138,0.0002242799,0.0008062084,0.0015211594,0.001690994,0.0005969071,0.0014075763],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021760853,0.00045000564,0.11932962,0.00067198335,0.00019654426,0.005023277,0.0030717584,0.09341155,0.2232331,0.3005535,0.020609068,0.23127359],"study_design_scores_gemma":[0.00022940413,0.0009089019,0.100054525,0.0001611133,0.000093728726,0.009730337,0.0015742369,0.48194492,0.09951574,0.22737841,0.078262985,0.00014571179],"about_ca_topic_score_codex":0.00042468234,"about_ca_topic_score_gemma":0.00016406667,"teacher_disagreement_score":0.0042932257,"about_ca_system_score_codex":0.00034482262,"about_ca_system_score_gemma":0.00021385083,"threshold_uncertainty_score":0.014362276},"labels":[],"label_agreement":null},{"id":"W4313244189","doi":"10.3847/1538-4357/acab5f","title":"Erratum: “The NANOGrav 12.5 yr Data Set: Polarimetry and Faraday Rotation Measures from Observations of Millisecond Pulsars with the Green Bank Telescope” (2022, ApJ, 926, 168)","year":2022,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Geophysics and Sensor Technology","field":"Engineering","cited_by":2,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; University of British Columbia","funders":"Science and Technology Facilities Council","keywords":"Physics; Polarimetry; Faraday effect; Millisecond pulsar; Pulsar; Astronomy; Telescope; Astrophysics; Rotation (mathematics); Green Bank Telescope; Magnetic field; Optics","score_opus":0.02368263136637339,"score_gpt":0.21211904649509358,"score_spread":0.1884364151287202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313244189","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0016061137,0.0010853295,0.000618807,0.042995784,0.9002758,0.000057819267,0.023737961,0.00101189,0.028610468],"genre_scores_gemma":[0.02115349,0.004495569,0.0043975604,0.104930416,0.12943062,0.00025128465,0.061011273,0.003570656,0.6707591],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9982893,0.00011616326,0.00028073322,0.00019652801,0.00096426567,0.00015300918],"domain_scores_gemma":[0.9912975,0.0012720269,0.0006479846,0.0006905376,0.005438996,0.00065309764],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013676259,0.0020624981,0.0012969318,0.004679101,0.0048703006,0.003980504,0.0017723899,0.0034947398,0.056832198],"category_scores_gemma":[0.012266681,0.0009769812,0.0010485187,0.003121115,0.0010631623,0.0021706375,0.0017966878,0.005806987,0.05628736],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000042459626,0.000013339508,0.00015295229,0.000033021108,0.0000054393217,0.000116026975,0.000012224968,0.00003400267,0.00010023301,0.00026119745,0.99705434,0.0021747479],"study_design_scores_gemma":[0.000037168473,0.000030805022,0.003947294,0.00012469504,0.000024965135,0.00017666459,0.000117800766,0.00015333772,0.00054855377,0.0006893259,0.99411017,0.00003932015],"about_ca_topic_score_codex":0.050037626,"about_ca_topic_score_gemma":0.06461156,"teacher_disagreement_score":0.056832198,"about_ca_system_score_codex":0.0031256387,"about_ca_system_score_gemma":0.0056974217,"threshold_uncertainty_score":0.1901226},"labels":[],"label_agreement":null},{"id":"W4313462466","doi":"10.3847/1538-4357/aca324","title":"Pre-main-sequence Brackett Emitters in the APOGEE DR17 Catalog: Line Strengths and Physical Properties of Accretion Columns","year":2022,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Lawrence Berkeley National Laboratory; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Vanderbilt University; Consejo Nacional de Ciencia y Tecnología; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; University of Portsmouth; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Radiative transfer; Accretion (finance); Ionization; Spectral line; Line (geometry); Emission spectrum; Stars; Main sequence; Astronomy; Ion; Geometry","score_opus":0.015961600240396164,"score_gpt":0.2572456825235011,"score_spread":0.24128408228310494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313462466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9466516,0.00041001578,0.00048278755,0.00003615532,0.0000058511555,0.000022270931,0.04904117,0.00021425581,0.0031358656],"genre_scores_gemma":[0.7932271,0.00071073417,0.0024301105,0.00006410638,0.000032257623,0.00009484787,0.19921096,0.00017023712,0.0040596644],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997938,0.000012149664,0.000025924155,0.00006162329,0.00006443135,0.000041960837],"domain_scores_gemma":[0.99843735,0.00012243519,0.00078779954,0.00024262915,0.00022303918,0.00018670881],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031870764,0.000377578,0.00028713426,0.0033815762,0.00019733868,0.00055584457,0.00038813415,0.0001621274,0.004845315],"category_scores_gemma":[0.00073708047,0.00013906497,0.00014011984,0.0030457783,0.000121194,0.00028343848,0.00055562664,0.00013183717,0.0028622292],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016011742,0.000040499854,0.95796496,0.00012153647,0.00007691358,0.00014705339,0.00024375858,0.00024636908,0.01057984,0.00027068285,0.009387922,0.020760313],"study_design_scores_gemma":[0.000014166847,0.000024924488,0.98773545,0.000016813827,0.000018710087,0.0002884278,0.00010110912,0.0002790613,0.001972637,0.00004850001,0.009493687,0.000006505836],"about_ca_topic_score_codex":0.004418441,"about_ca_topic_score_gemma":0.006587422,"teacher_disagreement_score":0.004845315,"about_ca_system_score_codex":0.00019886869,"about_ca_system_score_gemma":0.00020838519,"threshold_uncertainty_score":0.016209185},"labels":[],"label_agreement":null},{"id":"W4313580563","doi":"10.3847/1538-4357/aca47f","title":"Increasing Mass-to-flux Ratio from the Dense Core to the Protostellar Envelope around the Class 0 Protostar HH 211","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Ministry of Science and Technology, Taiwan; Academia Sinica","keywords":"Physics; Protostar; Ambipolar diffusion; Astrophysics; Magnetic field; Millimeter; Submillimeter Array; Flux (metallurgy); Magnetic flux; Polarization (electrochemistry); Star formation; Stars; Plasma","score_opus":0.02446149428320853,"score_gpt":0.26089518290095703,"score_spread":0.2364336886177485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313580563","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994072,0.00003987121,0.000115920295,0.000012703586,0.0000010251513,0.0000010255758,0.0000665249,0.000012613492,0.0003431544],"genre_scores_gemma":[0.99965215,0.000021548716,0.000074260905,0.000008534195,0.0000032852743,0.0000013223183,0.00015047367,0.000004209185,0.00008417271],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999696,0.0000020122238,0.0000014791038,0.000011367792,0.000008382739,0.0000072827584],"domain_scores_gemma":[0.9998474,0.000027627406,0.000044164306,0.000012283766,0.000021087471,0.000047373025],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000058496524,0.00014461299,0.00016048644,0.0006703113,0.0002583104,0.00032763113,0.00016659367,0.00016706677,0.0008282851],"category_scores_gemma":[0.00022287064,0.00013403373,0.00012660067,0.00028560343,0.00024384842,0.00017074037,0.00030176065,0.00020326664,0.00017297253],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004021408,0.00004952498,0.6362629,0.0000367736,0.00007263411,0.00069332815,0.00027650042,0.0009816468,0.3516386,0.00037701402,0.00025733892,0.008951599],"study_design_scores_gemma":[0.0000038731537,0.000019326635,0.995141,0.0000014006779,0.000008769595,0.00012132173,0.00007387251,0.00071104895,0.0037045954,0.0000529645,0.00015921987,0.0000025252868],"about_ca_topic_score_codex":0.0015874526,"about_ca_topic_score_gemma":0.0012920629,"teacher_disagreement_score":0.0015874526,"about_ca_system_score_codex":0.00024847826,"about_ca_system_score_gemma":0.00007411461,"threshold_uncertainty_score":0.0031564236},"labels":[],"label_agreement":null},{"id":"W4313580756","doi":"10.3847/1538-4357/aca46e","title":"The State of the Molecular Gas in Post-starburst Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; National Institutes of Natural Sciences; Max-Planck-Institut für Astrophysik; National Research Foundation of Korea; Directorate for Mathematical and Physical Sciences; University of Oxford; York University; U.S. Department of Energy; Smithsonian Institution; National Radio Astronomy Observatory; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Ohio State University; National Research Foundation; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; National Science Foundation; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Astrophysics; Galaxy; Star formation; Luminous infrared galaxy; Astronomy; Stars; Interstellar medium","score_opus":0.006176830452439878,"score_gpt":0.22572259391385696,"score_spread":0.21954576346141708,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313580756","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994301,0.000044978977,0.000038204664,0.000007415663,7.372588e-7,0.0000014018989,0.00010695019,0.0000049532373,0.00036533715],"genre_scores_gemma":[0.9995165,0.000018003451,0.000066105145,0.0000081058515,0.0000020259238,0.0000015960119,0.00019599948,0.0000013313016,0.00019026201],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999237,0.000006905475,0.0000043999235,0.000022291784,0.000013966294,0.000028755094],"domain_scores_gemma":[0.9995689,0.000038421505,0.00016933732,0.000033230688,0.0000674139,0.00012272531],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001318662,0.00008728965,0.00013481989,0.0005196713,0.00025187628,0.00046613233,0.0002143336,0.0002096437,0.0012038402],"category_scores_gemma":[0.00027140422,0.000073651856,0.00010747771,0.00037828268,0.00020393403,0.00020894446,0.00022317386,0.00019660773,0.00021812432],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007001418,0.000030832558,0.9731147,0.000009041557,0.000012339641,0.000066890745,0.00029806342,0.00006711036,0.023623997,0.000058644997,0.000068335656,0.0025799852],"study_design_scores_gemma":[3.9234615e-7,0.000010832482,0.9995616,5.3655185e-7,0.0000010125889,0.000017263814,0.00003444723,0.00003427483,0.00026193718,0.0000056099216,0.000071768525,3.6547564e-7],"about_ca_topic_score_codex":0.0056266063,"about_ca_topic_score_gemma":0.008081436,"teacher_disagreement_score":0.0056266063,"about_ca_system_score_codex":0.0003318878,"about_ca_system_score_gemma":0.00008500091,"threshold_uncertainty_score":0.011187732},"labels":[],"label_agreement":null},{"id":"W4313581322","doi":"10.3847/1538-4357/ac9f12","title":"Optimized Photometric Redshifts for the Cosmic Assembly Near-infrared Deep Extragalactic Legacy Survey (CANDELS)","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Redshift; Physics; Photometric redshift; Astrophysics; COSMIC cancer database; Outlier; Galaxy; Statistics; Mathematics","score_opus":0.022395826512622025,"score_gpt":0.2597627130714972,"score_spread":0.23736688655887514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4313581322","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.75354916,0.00035271564,0.22456248,0.00034154402,0.00005848465,0.00014944437,0.00983941,0.0061791367,0.0049676355],"genre_scores_gemma":[0.7217644,0.00008913091,0.2570313,0.00012745321,0.000032670196,0.00017208343,0.018494371,0.0009314309,0.001357065],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99799675,0.0005489201,0.00011330135,0.00046686135,0.0006600335,0.00021415463],"domain_scores_gemma":[0.994091,0.0014902336,0.0010025207,0.0016273465,0.001398225,0.00039069317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.009479214,0.0006383525,0.0006831074,0.0029222923,0.0007737619,0.0014638334,0.0010483514,0.00078995974,0.001454781],"category_scores_gemma":[0.019784434,0.0004729051,0.0011892839,0.0017942871,0.00037541927,0.000808575,0.0020719229,0.0008551592,0.00083486474],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076735864,0.00027711072,0.5160615,0.00018139445,0.0008309644,0.0001891285,0.0005114263,0.23776068,0.014625076,0.012920601,0.014102506,0.2017723],"study_design_scores_gemma":[0.000381686,0.00023979571,0.57349634,0.00010743583,0.0002897356,0.00024034818,0.00036994324,0.35458225,0.031763136,0.017930683,0.020333938,0.00026468522],"about_ca_topic_score_codex":0.014277424,"about_ca_topic_score_gemma":0.01820316,"teacher_disagreement_score":0.014277424,"about_ca_system_score_codex":0.001409677,"about_ca_system_score_gemma":0.0016544737,"threshold_uncertainty_score":0.05013144},"labels":[],"label_agreement":null},{"id":"W4315478396","doi":"10.3847/1538-4357/aca27e","title":"Meteorites and the RNA World: Synthesis of Nucleobases in Carbonaceous Planetesimals and the Role of Initial Volatile Content","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"H2020 European Research Council; H2020 Excellent Science; Natural Sciences and Engineering Research Council of Canada; Universität Heidelberg; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Deutsche Forschungsgemeinschaft; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology","keywords":"Planetesimal; Uracil; Thymine; Chondrite; Nucleobase; Meteorite; Cytosine; Chemistry; Hadean; Early Earth; Astrobiology; Guanine; Abiogenesis; Parent body; Solar System; DNA; Physics; Biochemistry; Mantle (geology)","score_opus":0.010755329030229223,"score_gpt":0.2239991851095931,"score_spread":0.21324385607936389,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4315478396","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98857725,0.0010748539,0.008086896,0.00010220952,0.000017620123,0.000010367388,0.00010529049,0.000045032637,0.0019804584],"genre_scores_gemma":[0.9980901,0.00023789161,0.0010801496,0.000007714049,0.0000034231082,0.00000602922,0.00004968773,0.000010070251,0.0005148392],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999397,0.0000076188235,0.0000030092756,0.000024944213,0.0000141746805,0.00001063855],"domain_scores_gemma":[0.9999062,0.000040116818,0.000019715942,0.000008587494,0.000013417027,0.000011934569],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013531819,0.00032877133,0.00024683247,0.0002186653,0.0002919515,0.0005838719,0.00035021667,0.00064539857,0.0007428362],"category_scores_gemma":[0.00042591177,0.00020354727,0.00031516457,0.00016833527,0.00035453757,0.00064875896,0.00025197573,0.00027407787,0.00015031722],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031766185,0.00017164428,0.034644224,0.00045514683,0.00010567045,0.00090002484,0.00028064576,0.55781215,0.37760156,0.015637,0.00021655345,0.011857758],"study_design_scores_gemma":[0.00003691543,0.00018104335,0.012950054,0.000022673852,0.00003335133,0.000160305,0.000110560504,0.90444684,0.07749521,0.002630933,0.0018978718,0.0000342411],"about_ca_topic_score_codex":0.007365693,"about_ca_topic_score_gemma":0.002502738,"teacher_disagreement_score":0.007365693,"about_ca_system_score_codex":0.0006565637,"about_ca_system_score_gemma":0.0003040707,"threshold_uncertainty_score":0.014645636},"labels":[],"label_agreement":null},{"id":"W4315490268","doi":"10.3847/1538-4357/acacfa","title":"Erratum: “VERTICO II: How H i-identified Environmental Mechanisms Affect the Molecular Gas in Cluster Galaxies” (2022, ApJ, 933, 10)","year":2023,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Royal Military College of Canada; McMaster University; Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Simons Foundation; National Natural Science Foundation of China; Canada Research Chairs","keywords":"Physics; Cluster (spacecraft); Astrophysics; Galaxy; Affect (linguistics); Galaxy cluster; Astronomy; Psychology; Communication","score_opus":0.0075971844011855725,"score_gpt":0.2149371105757874,"score_spread":0.20733992617460184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4315490268","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0005121803,0.001694831,0.0005542788,0.048226707,0.9303583,0.000019382996,0.0023089014,0.0004902409,0.015835226],"genre_scores_gemma":[0.018266324,0.007106926,0.0046213046,0.12984052,0.26810488,0.00012812973,0.007979691,0.0044087204,0.5595434],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988662,0.00011307577,0.00016241873,0.00021507793,0.0005541119,0.000089129855],"domain_scores_gemma":[0.9935812,0.0010258869,0.00042559134,0.0004943605,0.0038934804,0.0005795324],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016551662,0.0017650678,0.0009327244,0.0019735075,0.0039025538,0.003924335,0.0019307128,0.0031689391,0.058688156],"category_scores_gemma":[0.012126063,0.00081773056,0.0012211865,0.0017905837,0.0016830324,0.0027539006,0.0017620794,0.007566416,0.05561889],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000014531692,0.0000034848895,0.00008515781,0.000028025237,0.0000037443394,0.00006174153,0.000016079457,0.000013071957,0.000054161454,0.00037138158,0.99671113,0.0026374422],"study_design_scores_gemma":[0.000019148152,0.000014455108,0.0025194688,0.00017876874,0.000030333045,0.0002598548,0.00012934233,0.00009976782,0.0003775781,0.0014548315,0.9948842,0.00003216191],"about_ca_topic_score_codex":0.040152226,"about_ca_topic_score_gemma":0.05762428,"teacher_disagreement_score":0.058688156,"about_ca_system_score_codex":0.0028105914,"about_ca_system_score_gemma":0.0038966767,"threshold_uncertainty_score":0.19633144},"labels":[],"label_agreement":null},{"id":"W4315785820","doi":"10.3847/1538-4357/aca4d2","title":"On the Origin of the North Celestial Pole Loop","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Loop (graph theory); Celestial mechanics; Astronomy; Astrophysics","score_opus":0.015722907231075025,"score_gpt":0.24343338257226477,"score_spread":0.22771047534118974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4315785820","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97984695,0.0003209318,0.0066916933,0.0004929959,0.00005383391,0.0000102875,0.00012243378,0.00017820262,0.012282562],"genre_scores_gemma":[0.9986039,0.00003010799,0.0009041874,0.000016977157,0.000009422791,0.0000016841853,0.00005826137,0.000011012347,0.00036448048],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999056,0.000013845311,0.0000017241821,0.000029361132,0.000030220324,0.000019203473],"domain_scores_gemma":[0.9997633,0.000042360498,0.00004156816,0.000037944992,0.000050890903,0.000063914515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013400537,0.00009554402,0.00016091917,0.00033011558,0.00043991653,0.000958896,0.0002610815,0.00031736805,0.0020638383],"category_scores_gemma":[0.0010086414,0.0001242558,0.00009916227,0.0002112729,0.00072115887,0.00051627355,0.000534844,0.00045503431,0.00023125121],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010954322,0.00014868092,0.5608333,0.00012972967,0.000056187655,0.0048765033,0.0059407717,0.046894383,0.13725832,0.12721178,0.007854266,0.10770064],"study_design_scores_gemma":[0.00010962236,0.00022747231,0.6870567,0.000100203426,0.000029390805,0.001661474,0.0027571663,0.1835529,0.012579777,0.036335096,0.07549735,0.00009276719],"about_ca_topic_score_codex":0.008316345,"about_ca_topic_score_gemma":0.004302128,"teacher_disagreement_score":0.008316345,"about_ca_system_score_codex":0.0005950826,"about_ca_system_score_gemma":0.00023264912,"threshold_uncertainty_score":0.016535878},"labels":[],"label_agreement":null},{"id":"W4316015670","doi":"10.3847/1538-4357/aca1b1","title":"Gap-opening Planets Make Dust Rings Wider","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Academia Sinica; Alfred P. Sloan Foundation","keywords":"Physics; Planet; Astrophysics; Turbulence; Planetary system; Advection; Astronomy; Mechanics","score_opus":0.020106256946412472,"score_gpt":0.2531181730916922,"score_spread":0.23301191614527975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4316015670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984037,0.000059671438,0.0009368133,0.00003331913,0.000006193056,0.0000011450736,0.000024936033,0.000033478354,0.0005007017],"genre_scores_gemma":[0.99971324,0.000016204203,0.00019647753,0.0000061564197,0.0000015676898,5.312023e-7,0.000011921233,0.0000039637844,0.000049882576],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994993,0.000007708696,0.0000027062906,0.000016121186,0.0000074589802,0.000015955753],"domain_scores_gemma":[0.99956805,0.00013180826,0.00008829487,0.00006893956,0.00002211761,0.00012073912],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013583298,0.00013232305,0.00019013285,0.00014421901,0.00027395168,0.0005419664,0.00022659723,0.00036446704,0.001208894],"category_scores_gemma":[0.00070387416,0.00016420361,0.0003290454,0.000102193386,0.00039977502,0.0005500477,0.0006066623,0.00030586697,0.00011494258],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007964045,0.0002948282,0.22580072,0.00025966862,0.00039671824,0.0024562457,0.0010046572,0.39567322,0.34154138,0.015745351,0.0016585218,0.014372237],"study_design_scores_gemma":[0.000099611556,0.00033735362,0.26826614,0.00003272306,0.0001803569,0.001216465,0.00076450227,0.6588069,0.052505665,0.013571768,0.0041466663,0.00007180926],"about_ca_topic_score_codex":0.0005872415,"about_ca_topic_score_gemma":0.00056335976,"teacher_disagreement_score":0.001208894,"about_ca_system_score_codex":0.00019557266,"about_ca_system_score_gemma":0.00009729272,"threshold_uncertainty_score":0.004044175},"labels":[],"label_agreement":null},{"id":"W4317038228","doi":"10.3847/1538-4357/aca657","title":"Dependence of Chemical Abundance on the Cosmic-Ray Ionization Rate in IC 348","year":2023,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Centre for Interdisciplinary Research in Rehabilitation; University of California, Los Angeles; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; China Postdoctoral Science Foundation; California Institute of Technology; Academia Sinica; National Natural Science Foundation of China; Jet Propulsion Laboratory; Deutsche Forschungsgemeinschaft","keywords":"Physics; Ionization; Astrophysics; Stars; Abundance (ecology); Analytical Chemistry (journal); Line (geometry); Ion; Molecular cloud; Abundance of the chemical elements; Extinction (optical mineralogy); Chemistry; Optics","score_opus":0.015252429618842725,"score_gpt":0.24384100185728763,"score_spread":0.22858857223844492,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4317038228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99915123,0.00002575461,0.00011500267,0.000009794981,4.4425389e-7,0.0000021280448,0.00012539083,0.000022074111,0.00054818945],"genre_scores_gemma":[0.99967563,0.000011079838,0.00004463804,0.0000031204409,5.3702473e-7,0.0000012766365,0.00018740214,0.0000036989702,0.000072573916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991465,0.0000069589287,0.000002785891,0.000030046822,0.000014296848,0.000031261334],"domain_scores_gemma":[0.99962354,0.00010810113,0.00009326777,0.00004058148,0.00006337604,0.000071039154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010832346,0.00023688063,0.00018301583,0.0005822828,0.00016322937,0.000388707,0.00025144868,0.00023815992,0.0009536049],"category_scores_gemma":[0.00072736735,0.00019137528,0.00014252329,0.00032484377,0.00021173147,0.00019470765,0.00024889747,0.00023212754,0.00020339285],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003762329,0.000046038167,0.86346865,0.000025321586,0.000073397234,0.00023600117,0.00010439842,0.009681757,0.11760067,0.00031937598,0.00033784757,0.0077303853],"study_design_scores_gemma":[0.000005397966,0.00006934051,0.9848605,0.0000032629816,0.000015463476,0.0001027501,0.000056991834,0.009560991,0.0049886764,0.00007760912,0.0002514425,0.000007581994],"about_ca_topic_score_codex":0.0110408515,"about_ca_topic_score_gemma":0.009559706,"teacher_disagreement_score":0.0110408515,"about_ca_system_score_codex":0.00048020636,"about_ca_system_score_gemma":0.00011062553,"threshold_uncertainty_score":0.021953225},"labels":[],"label_agreement":null},{"id":"W4317214163","doi":"10.3847/1538-4357/aca768","title":"SDSS-IV MaNGA: How Galaxy Interactions Influence Active Galactic Nuclei","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Accretion (finance); Galaxy formation and evolution; Astronomy","score_opus":0.009950916647045453,"score_gpt":0.23532604705283108,"score_spread":0.22537513040578563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4317214163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99890745,0.00006796816,0.00010156049,0.00004323147,0.0000018841192,0.0000023620728,0.00031056412,0.000016656837,0.00054823054],"genre_scores_gemma":[0.9995198,0.000011059216,0.000095850075,0.000008207428,0.0000029346181,0.0000018473206,0.0002634481,0.000008137223,0.00008881039],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99956983,0.00018750674,0.000015843643,0.00011481027,0.00005504104,0.000056955065],"domain_scores_gemma":[0.9980921,0.00074287987,0.0005104373,0.00019084712,0.00013882662,0.00032489927],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00073761906,0.00019524437,0.00027127538,0.0006056683,0.00036366357,0.00071121915,0.0003507384,0.00017938338,0.0010272597],"category_scores_gemma":[0.002153331,0.00013739709,0.00026468263,0.0006022605,0.00035423876,0.0003794558,0.00054966804,0.00018270705,0.00026552178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009760351,0.000023991897,0.99229103,0.000013495469,0.00008036107,0.00006172919,0.00013499259,0.0017379228,0.0030146872,0.0002934111,0.0002633642,0.001987528],"study_design_scores_gemma":[0.0000053369163,0.000024684876,0.9939122,0.0000035522278,0.00001848946,0.000027631808,0.00012780451,0.005044093,0.00040285988,0.00011304627,0.0003156905,0.000004687604],"about_ca_topic_score_codex":0.014144312,"about_ca_topic_score_gemma":0.017017137,"teacher_disagreement_score":0.014144312,"about_ca_system_score_codex":0.0006092181,"about_ca_system_score_gemma":0.0002558854,"threshold_uncertainty_score":0.028123915},"labels":[],"label_agreement":null},{"id":"W4317553566","doi":"10.3847/1538-4357/aca655","title":"Cool, Luminous, and Highly Variable Stars in the Magellanic Clouds. II. Spectroscopic and Environmental Analysis of Thorne–Żytkow Object and Super-AGB Star Candidates","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; University of Toronto; National Aeronautics and Space Administration; Canada Research Chairs; Canadian Institute for Advanced Research; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Stars; Red supergiant; Supergiant; Large Magellanic Cloud; Supernova; Nucleosynthesis; Astronomy; Population; Neutron star; Asymptotic giant branch; Stellar evolution","score_opus":0.00597850761453164,"score_gpt":0.20444787295861994,"score_spread":0.1984693653440883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4317553566","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997538,0.000028303748,0.000022157996,0.0000024220456,3.5842362e-7,0.0000017660124,0.000059877275,8.254872e-7,0.00013049146],"genre_scores_gemma":[0.9996413,0.000018225803,0.000044574655,0.0000024941062,0.0000010792556,0.0000014643606,0.00022119118,6.6072556e-7,0.00006895054],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987483,0.000011001847,0.000011747176,0.000040225663,0.000025137912,0.000036943784],"domain_scores_gemma":[0.99962664,0.000038099482,0.00013685938,0.000022126886,0.00004155899,0.00013470328],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015292225,0.00015351789,0.00020046653,0.0017813396,0.00044881523,0.00042202705,0.00018285205,0.00015852311,0.00085888745],"category_scores_gemma":[0.000405777,0.000100471414,0.00016374269,0.0007802132,0.0002679052,0.0002103882,0.00048812997,0.00014077485,0.00023924552],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000032411157,0.000010244085,0.99563193,0.0000037710693,0.000007056313,0.00005774129,0.00007544132,0.000032169453,0.003072819,0.000017426326,0.000011853456,0.0010470969],"study_design_scores_gemma":[6.8662195e-7,0.000015202441,0.99951446,6.9143863e-7,0.0000023146702,0.00009489419,0.00010969856,0.00005073046,0.00016266244,0.000007661594,0.000040401705,5.8793444e-7],"about_ca_topic_score_codex":0.0057184114,"about_ca_topic_score_gemma":0.008571344,"teacher_disagreement_score":0.0057184114,"about_ca_system_score_codex":0.00022971403,"about_ca_system_score_gemma":0.00016309727,"threshold_uncertainty_score":0.011370242},"labels":[],"label_agreement":null},{"id":"W4317951747","doi":"10.3847/1538-4357/aca7ca","title":"The Pan-STARRS1 z &gt; 5.6 Quasar Survey. III. The z ≈ 6 Quasar Luminosity Function","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University; Space Telescope Science Institute; Eötvös Loránd Tudományegyetem; California Institute of Technology; European Commission; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; National Central University; Gordon and Betty Moore Foundation; Smithsonian Institution; Durham University; Planetary Science Division; Science Mission Directorate; Universities Space Research Association; National Science Foundation","keywords":"Quasar; Physics; Astrophysics; Luminosity function; Luminosity; Approx; Light curve; Redshift; Galaxy","score_opus":0.014523939988257574,"score_gpt":0.22487195540632665,"score_spread":0.21034801541806908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4317951747","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9832682,0.0002723531,0.0007589745,0.00015043806,0.0000066506973,0.000015531941,0.011553422,0.00016748281,0.0038070052],"genre_scores_gemma":[0.97676325,0.00017884462,0.0008995626,0.000048683927,0.000017881657,0.00001647197,0.019816214,0.00006575073,0.0021932896],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978024,0.000038049522,0.000013285434,0.000055284123,0.00007124714,0.000041922347],"domain_scores_gemma":[0.9992754,0.00005454146,0.00032549826,0.00008612171,0.0001240168,0.00013450705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006137249,0.00026192196,0.00020844996,0.0013412628,0.000141355,0.0003663651,0.00027456356,0.00014080318,0.0034276275],"category_scores_gemma":[0.0007681575,0.00012290958,0.00026438702,0.0007595732,0.00013204261,0.0003803018,0.00043765057,0.00016710263,0.0012499243],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014602393,0.000025414874,0.96918565,0.00006134931,0.000056195862,0.00010284694,0.00018681806,0.0005660786,0.0039060297,0.00037257772,0.0045994553,0.020791601],"study_design_scores_gemma":[0.000005275722,0.0000276922,0.9963012,0.000004545086,0.000010485564,0.00010974016,0.000045796354,0.0004801683,0.0005407904,0.000037145386,0.0024345524,0.0000025472777],"about_ca_topic_score_codex":0.007866478,"about_ca_topic_score_gemma":0.012201935,"teacher_disagreement_score":0.007866478,"about_ca_system_score_codex":0.00023025235,"about_ca_system_score_gemma":0.00011398991,"threshold_uncertainty_score":0},"labels":[],"label_agreement":null},{"id":"W4317951797","doi":"10.3847/1538-4357/acb338","title":"Erratum: “On the Use of Field RR Lyrae as Galactic Probes. V. Optical and Radial Velocity Curve Templates” (2021, ApJ, 919, 85)","year":2023,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Radial velocity; Astrophysics; RR Lyrae variable; Field (mathematics); Light curve; Astronomy; Galaxy; Stars; Globular cluster","score_opus":0.034431685673425416,"score_gpt":0.28465236468606364,"score_spread":0.2502206790126382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4317951797","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0011782974,0.0022577476,0.0011302575,0.08174448,0.85940796,0.000089510206,0.010060411,0.0012947059,0.042836666],"genre_scores_gemma":[0.013668145,0.0057108765,0.006949817,0.1487279,0.10831136,0.00022967775,0.016705155,0.0029096592,0.6967873],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99842083,0.00015941636,0.0003093407,0.0001948388,0.0007932038,0.00012243993],"domain_scores_gemma":[0.98912185,0.0018282321,0.00053482834,0.0007899759,0.0071212277,0.00060383923],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017776154,0.0015237463,0.00093036925,0.002223441,0.0037170264,0.002996046,0.0018507043,0.0038392816,0.050763626],"category_scores_gemma":[0.016780974,0.000796799,0.0009882193,0.0018401073,0.0010073608,0.0018276768,0.0013335345,0.005939785,0.059734352],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000028504024,0.0000056475633,0.00006950601,0.000023863864,0.0000025875818,0.00007899887,0.000009398867,0.000017465652,0.00006531029,0.00025862938,0.99686676,0.0025732976],"study_design_scores_gemma":[0.000029335548,0.000022378006,0.0026232707,0.00018736214,0.000023019918,0.00022441169,0.000087833796,0.00013762485,0.0007089241,0.0008881654,0.99503124,0.00003647523],"about_ca_topic_score_codex":0.053878624,"about_ca_topic_score_gemma":0.07196607,"teacher_disagreement_score":0.053878624,"about_ca_system_score_codex":0.0028304942,"about_ca_system_score_gemma":0.0042836643,"threshold_uncertainty_score":0.16982126},"labels":[],"label_agreement":null},{"id":"W4318040552","doi":"10.3847/1538-4357/aca5fa","title":"The DESI Survey Validation: Results from Visual Inspection of Bright Galaxies, Luminous Red Galaxies, and Emission-line Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"CCD and CMOS Imaging Sensors","field":"Engineering","cited_by":73,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"High Energy Physics; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; National Taiwan University; Ministerio de Ciencia e Innovación; National Science Foundation; Consejo Nacional de Ciencia y Tecnología; Gordon and Betty Moore Foundation; U.S. Department of Energy; Ministry of Education, India; Division of Astronomical Sciences; Science and Technology Facilities Council","keywords":"Physics; Redshift; Galaxy; Astrophysics; Luminous infrared galaxy; Astronomy","score_opus":0.016691025190763785,"score_gpt":0.2394759720975229,"score_spread":0.2227849469067591,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318040552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98148465,0.00022115836,0.009989535,0.00006484766,0.000028875713,0.000088439345,0.00412396,0.0012484109,0.0027501264],"genre_scores_gemma":[0.9780115,0.00005007441,0.009139541,0.00006723331,0.000009176615,0.000035877467,0.011328912,0.00023103421,0.0011266146],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9969963,0.00064009696,0.0002563661,0.0007340162,0.0010689716,0.00030432205],"domain_scores_gemma":[0.9907589,0.0019645751,0.0013311642,0.0016357821,0.0037821694,0.0005274106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038536154,0.0007828873,0.00046462187,0.0028597522,0.0005948786,0.0010717906,0.00058314926,0.00080861506,0.00068917236],"category_scores_gemma":[0.008226382,0.0002947921,0.00068071653,0.0011861873,0.0005438005,0.0006423432,0.0012808089,0.00033408808,0.00066642597],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014309216,0.0005953628,0.8141275,0.00032020023,0.00047715788,0.00034296478,0.0010158693,0.020143952,0.06440895,0.00069470244,0.0064350218,0.09000736],"study_design_scores_gemma":[0.000067718756,0.00036754744,0.8913068,0.000047453916,0.00011277363,0.0003235328,0.00043642448,0.05553976,0.04580187,0.00027019365,0.005661315,0.00006464801],"about_ca_topic_score_codex":0.009177984,"about_ca_topic_score_gemma":0.009427064,"teacher_disagreement_score":0.009177984,"about_ca_system_score_codex":0.00058908446,"about_ca_system_score_gemma":0.00027449994,"threshold_uncertainty_score":0.02038014},"labels":[],"label_agreement":null},{"id":"W4318068627","doi":"10.3847/1538-4357/aca7c2","title":"A Framework for Obtaining Accurate Posteriors of Strong Gravitational Lensing Parameters with Flexible Priors and Implicit Likelihoods Using Density Estimation","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; Fonds de recherche du Québec; Agence Nationale de la Recherche","keywords":"Prior probability; Gravitational lens; Algorithm; Posterior probability; Bayesian inference; Bayesian probability; Inference; Point estimation; Physics; Computer science; Artificial intelligence; Statistics; Astrophysics; Mathematics; Galaxy","score_opus":0.02561300295988669,"score_gpt":0.28647854484471513,"score_spread":0.26086554188482847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318068627","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.013876396,0.000116259565,0.98469603,0.0002577971,0.000011545261,0.000018521449,0.00009464743,0.00039142524,0.0005374304],"genre_scores_gemma":[0.48682517,0.000369784,0.50882107,0.00026127507,0.000121118355,0.00021103524,0.00059089507,0.00043321072,0.0023663738],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99843603,0.00069846225,0.00006581885,0.00024310201,0.00042624248,0.00013031674],"domain_scores_gemma":[0.98910683,0.007882858,0.00070842134,0.0011437715,0.0008620369,0.00029610205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.005233728,0.0013181788,0.0013156552,0.0014704354,0.000735691,0.0016879435,0.003918669,0.0016698923,0.0034178765],"category_scores_gemma":[0.031549606,0.0017149429,0.0010963968,0.0009914015,0.0028407262,0.005346313,0.003605663,0.004070389,0.0006693575],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007382322,0.000032829506,0.0008549368,0.000050115188,0.00003390666,0.000049145878,0.000062364365,0.93330127,0.0009912949,0.045933995,0.00060529297,0.018011067],"study_design_scores_gemma":[0.0000070226547,0.000004378037,0.000063782165,0.0000043208215,0.0000020262487,0.0000057580387,0.0000021830217,0.9809399,0.00024540257,0.018600654,0.00012017144,0.000004355125],"about_ca_topic_score_codex":0.0141036045,"about_ca_topic_score_gemma":0.011492776,"teacher_disagreement_score":0.0141036045,"about_ca_system_score_codex":0.0024785732,"about_ca_system_score_gemma":0.0023769294,"threshold_uncertainty_score":0.028042972},"labels":[],"label_agreement":null},{"id":"W4318485470","doi":"10.3847/1538-4357/acaa38","title":"Models of Rotating Infall for the B335 Protostar","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; National Research Foundation of Korea; National Science Council; National Research Foundation; National Institutes of Natural Sciences; European Space Agency; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Protostar; Astrophysics; Astronomy; Stars; Star formation","score_opus":0.02336023548412123,"score_gpt":0.24825447309069198,"score_spread":0.22489423760657076,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318485470","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94376826,0.00037897626,0.041252486,0.0005335655,0.00002752857,0.000036515372,0.00039685756,0.0002201241,0.013385593],"genre_scores_gemma":[0.9960873,0.000114719136,0.0022398168,0.000027425618,0.000010217982,0.000021891065,0.00012976615,0.000021418738,0.0013474103],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992776,0.000023932665,0.0000035732946,0.00001600676,0.000012244471,0.000016479817],"domain_scores_gemma":[0.9997558,0.00005363691,0.00006932148,0.000018133567,0.0000276101,0.00007535993],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024473606,0.0004599811,0.0003090886,0.00037417692,0.0005621588,0.00097492436,0.0009494993,0.0005938457,0.0017393477],"category_scores_gemma":[0.0006647342,0.0003099092,0.0006592645,0.00028796383,0.0006169116,0.00053539616,0.00053916755,0.00031342098,0.00039535973],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000118577875,0.00002986985,0.009214599,0.000020114003,0.000040299637,0.00030594983,0.00015851409,0.96496695,0.0019920578,0.019754434,0.00046737812,0.0029313061],"study_design_scores_gemma":[0.00003507494,0.000040916133,0.003884518,0.000007745832,0.000014982372,0.00007466209,0.000048151072,0.989971,0.00013739402,0.005009379,0.00076111616,0.000015028049],"about_ca_topic_score_codex":0.028009336,"about_ca_topic_score_gemma":0.010772593,"teacher_disagreement_score":0.028009336,"about_ca_system_score_codex":0.0012531142,"about_ca_system_score_gemma":0.00045102334,"threshold_uncertainty_score":0.055692613},"labels":[],"label_agreement":null},{"id":"W4318698665","doi":"10.3847/1538-4357/aca614","title":"Breaking Degeneracies in Formation Histories by Measuring Refractory Content in Gas Giants","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Space Telescope Science Institute","keywords":"Exoplanet; Physics; Gas giant; Giant planet; Planet; Astrophysics; Accretion (finance); Metallicity; Astrobiology; Refractory (planetary science); Hot Jupiter; Terrestrial planet; Protoplanetary disk; Astrochemistry; Silicate; Atmospheric escape; Planetary system; Astronomy; Stars; Interstellar medium; Galaxy","score_opus":0.03624959497788782,"score_gpt":0.2213804818204463,"score_spread":0.1851308868425585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318698665","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979371,0.0001694772,0.0010565176,0.0000081668695,0.0000011083403,0.00000376755,0.00017093304,0.000030110969,0.0006228436],"genre_scores_gemma":[0.99875593,0.00006103856,0.0008681371,0.000010450318,0.0000017589797,0.000004731632,0.0001722474,0.00000787987,0.000117881784],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998809,0.000016903055,0.000009129696,0.00004964452,0.00002344254,0.00001982266],"domain_scores_gemma":[0.99936,0.0001560797,0.0002750648,0.00007366316,0.000058685382,0.00007641851],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038863235,0.0002635158,0.00021017466,0.0011933954,0.00027593182,0.00063405174,0.0003901136,0.0003196007,0.00043034577],"category_scores_gemma":[0.00097304955,0.00018987703,0.00013481936,0.000561326,0.00039148325,0.0005031291,0.00053096784,0.00019692986,0.00012556276],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004049214,0.000023993965,0.8019498,0.000042275857,0.0001478673,0.00012648135,0.00049321924,0.0021596814,0.17719325,0.00046895182,0.00011367173,0.016875893],"study_design_scores_gemma":[0.000009881795,0.00011120775,0.95573974,0.00001359058,0.000065266955,0.00027128076,0.00032469895,0.007551645,0.034347665,0.00076152623,0.0007871193,0.00001633896],"about_ca_topic_score_codex":0.0024774782,"about_ca_topic_score_gemma":0.0033735796,"teacher_disagreement_score":0.0024774782,"about_ca_system_score_codex":0.00028352227,"about_ca_system_score_gemma":0.00008311647,"threshold_uncertainty_score":0.0049260855},"labels":[],"label_agreement":null},{"id":"W4318815871","doi":"10.3847/1538-4357/aca899","title":"Study of Radio Transients from the Quiet Sun during an Extremely Quiet Time","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Department of Atomic Energy, Government of India; Curtin University of Technology; Astronomy Australia Limited; National Cancer Research Institute; Commonwealth Scientific and Industrial Research Organisation; Government of Western Australia; National Science Foundation","keywords":"QUIET; Physics; Astronomy; Astrophysics","score_opus":0.013401058584745891,"score_gpt":0.23777373604804958,"score_spread":0.2243726774633037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318815871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959389,0.00019812916,0.0018209629,0.000027137597,0.000013196629,0.000009557642,0.00027580798,0.000046109195,0.0016701787],"genre_scores_gemma":[0.9977894,0.000078754696,0.0010597738,0.000022816925,0.00003318083,0.000007116797,0.0006186446,0.000020323268,0.00036990858],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998908,0.000011850752,0.000007284081,0.00003545909,0.00003198388,0.0000226078],"domain_scores_gemma":[0.99937683,0.00015754972,0.0001936184,0.00006199343,0.00009215315,0.00011787534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024362741,0.00016563272,0.0002483146,0.001641279,0.00032147547,0.00038814195,0.00026561038,0.00024081157,0.0011924958],"category_scores_gemma":[0.0005563868,0.000099785575,0.00018224666,0.0007740912,0.00021474046,0.00028211312,0.00040084086,0.0002893244,0.00031797166],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011047977,0.00026600726,0.652692,0.0002440638,0.00024227584,0.0030458963,0.0012239182,0.0022724716,0.28115764,0.001497123,0.001442223,0.054811563],"study_design_scores_gemma":[0.00001645564,0.00019435036,0.98470944,0.000014520086,0.000050719533,0.0009508639,0.00027050584,0.0024267202,0.008232028,0.00027285088,0.002841896,0.00001966753],"about_ca_topic_score_codex":0.0006551519,"about_ca_topic_score_gemma":0.0011749241,"teacher_disagreement_score":0.001641279,"about_ca_system_score_codex":0.00010947059,"about_ca_system_score_gemma":0.000063366155,"threshold_uncertainty_score":0.003989339},"labels":[],"label_agreement":null},{"id":"W4318897514","doi":"10.3847/1538-4357/aca8aa","title":"Galaxy Spin Classification. I. Z-wise versus S-wise Spirals with the Chirality Equivariant Residual Network","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Perimeter Institute; Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics","funders":"High Energy Physics; National Science Fund for Distinguished Young Scholars; Jet Propulsion Laboratory; Office of Science; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Canadian Institute for Advanced Research; Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China; Chinese Academy of Sciences; National Aeronautics and Space Administration; U.S. Department of Energy; California Institute of Technology; University of Sussex; Division of Astronomical Sciences; Alexander von Humboldt-Stiftung; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Sigma; Astronomy","score_opus":0.027787161610138465,"score_gpt":0.25902377142333854,"score_spread":0.23123660981320007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318897514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9278674,0.0007835565,0.05817478,0.0014858396,0.00015633299,0.000067829336,0.0017332354,0.001847686,0.007883261],"genre_scores_gemma":[0.98775023,0.00007798247,0.0085333465,0.000096869044,0.000029703036,0.000012896156,0.0018585444,0.00004301503,0.0015973619],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996877,0.00009181087,0.00001463159,0.00009294113,0.000044396664,0.00006844605],"domain_scores_gemma":[0.9988996,0.00038419332,0.00015249026,0.0002175302,0.00024334085,0.00010278752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010104481,0.000685189,0.0003588375,0.0008007987,0.0003149573,0.00094592094,0.0007614071,0.00072876987,0.0014542581],"category_scores_gemma":[0.0041446667,0.00015769798,0.00043064883,0.00042665092,0.0006422018,0.00090036384,0.0006648913,0.000784062,0.00054043485],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023083198,0.00041383525,0.16880815,0.00028020778,0.0002675701,0.00032283075,0.00026055585,0.4710347,0.019148264,0.011784033,0.016904803,0.30846667],"study_design_scores_gemma":[0.00001537046,0.00006834603,0.0060713277,0.000019128664,0.00002163293,0.000039193175,0.000047021047,0.9842684,0.00496201,0.0035817795,0.0008942024,0.000011444217],"about_ca_topic_score_codex":0.009558451,"about_ca_topic_score_gemma":0.009597334,"teacher_disagreement_score":0.009558451,"about_ca_system_score_codex":0.0008039579,"about_ca_system_score_gemma":0.00043446297,"threshold_uncertainty_score":0.019005597},"labels":[],"label_agreement":null},{"id":"W4318898040","doi":"10.3847/1538-4357/acac82","title":"Ghost in the Shell: Evidence for Past Active Galactic Nucleus Activities in NGC 5195 from a Newly Discovered Large-scale Ionized Structure","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Galaxy","score_opus":0.014315538142868319,"score_gpt":0.2527155356506285,"score_spread":0.23839999750776017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318898040","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99887925,0.00006211942,0.00010842202,0.000013565003,0.0000015279985,0.0000023767159,0.000064530745,0.000009922789,0.00085826195],"genre_scores_gemma":[0.9997198,0.00001279264,0.000076237,0.0000062112167,0.0000016804424,6.8057693e-7,0.00007638,0.0000010619137,0.00010514528],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994206,0.0000036093072,0.0000054154225,0.00001787883,0.000015000708,0.000016025977],"domain_scores_gemma":[0.99976057,0.000034187007,0.00008064419,0.000036946043,0.000016026657,0.000071625116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000093962124,0.00012075265,0.000104250605,0.0006018875,0.00026395483,0.0005390982,0.0002185396,0.00017445066,0.0016233703],"category_scores_gemma":[0.0003787675,0.00009217962,0.0001330696,0.0003363656,0.00032940385,0.00022146008,0.0004443465,0.0001385361,0.0001754472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018326583,0.000050700466,0.9164312,0.000031419146,0.000054050404,0.0045960094,0.0011538502,0.0002413102,0.066140175,0.0005083503,0.0003002656,0.010309442],"study_design_scores_gemma":[0.0000057808948,0.000038265083,0.99482465,0.000007863029,0.000016882936,0.0014998048,0.00032063475,0.00020563017,0.0020688986,0.00008959317,0.0009176791,0.0000042514203],"about_ca_topic_score_codex":0.0065297526,"about_ca_topic_score_gemma":0.0066217664,"teacher_disagreement_score":0.0065297526,"about_ca_system_score_codex":0.00029842526,"about_ca_system_score_gemma":0.000083221006,"threshold_uncertainty_score":0.012983501},"labels":[],"label_agreement":null},{"id":"W4318997029","doi":"10.3847/1538-4357/acae88","title":"Polarization Properties of the Weakly Magnetized Neutron Star X-Ray Binary GS 1826–238 in the High Soft State","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Russian Science Foundation; Agenzia Spaziale Italiana; Istituto Nazionale di Astrofisica; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Neutron star; Astrophysics; Polarization (electrochemistry); Polarimetry; Binary number; Monte Carlo method; X-ray binary; Computational physics; Scattering; Optics","score_opus":0.01338979549603782,"score_gpt":0.20814408741183657,"score_spread":0.19475429191579874,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318997029","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986708,0.00004088222,0.00012339087,0.000016420345,0.0000017091733,0.0000018627877,0.00011888723,0.000009848557,0.0010162545],"genre_scores_gemma":[0.99953663,0.000012495021,0.000055174485,0.00000472766,0.0000016544557,0.0000011662706,0.00021327409,0.000003913231,0.00017101366],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999285,0.000009900479,0.0000033469819,0.000026913527,0.000015921787,0.000015402813],"domain_scores_gemma":[0.9998105,0.00004104865,0.000054942313,0.00002150015,0.000026930427,0.000045102817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023965395,0.00021006809,0.0002746984,0.0004315772,0.00034294263,0.0007117755,0.00015564673,0.00022898147,0.0012116648],"category_scores_gemma":[0.0004153718,0.00020805164,0.00012997704,0.0003086204,0.00038423383,0.00020903411,0.00045117576,0.00027180868,0.00025188204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019439127,0.00018057287,0.57580864,0.000096751355,0.0001778722,0.0016357776,0.00067902915,0.021123167,0.38680714,0.003011773,0.00089354644,0.0076418617],"study_design_scores_gemma":[0.00010138796,0.00029171046,0.9384298,0.000014709355,0.000047914433,0.00040002007,0.0003472698,0.028352672,0.029634343,0.0008752416,0.0014628485,0.00004210041],"about_ca_topic_score_codex":0.002095866,"about_ca_topic_score_gemma":0.0015772202,"teacher_disagreement_score":0.002095866,"about_ca_system_score_codex":0.0004122971,"about_ca_system_score_gemma":0.00011354058,"threshold_uncertainty_score":0.004167378},"labels":[],"label_agreement":null},{"id":"W4318997122","doi":"10.3847/1538-4357/ac8481","title":"Patchy Kinetic Sunyaev–Zel’dovich Effect with Controlled Reionization History and Morphology","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Reionization; Physics; Redshift; South Pole Telescope; Halo; Astrophysics; Galaxy","score_opus":0.004707112316948316,"score_gpt":0.18994170315488174,"score_spread":0.18523459083793342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4318997122","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96195936,0.0002579546,0.02364834,0.00037938685,0.00007536418,0.000049100352,0.0004156912,0.0006518163,0.012563106],"genre_scores_gemma":[0.9969926,0.000042884767,0.0017542499,0.00006563826,0.000012345349,0.000024026438,0.00007198133,0.00012061331,0.0009156258],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998673,0.000021336977,0.0000047308254,0.00002850779,0.000022157701,0.000055877215],"domain_scores_gemma":[0.99950397,0.000129978,0.0001298608,0.00008343476,0.000032957872,0.00011975141],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029289772,0.0003711536,0.00059060066,0.000309238,0.00037106214,0.000745669,0.0012437328,0.00057818706,0.0039062854],"category_scores_gemma":[0.0014128509,0.00028048817,0.00058652885,0.00021145467,0.00081812066,0.00062231475,0.0010193241,0.0006484835,0.0002786291],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002560212,0.000097560034,0.013214043,0.00007431049,0.00010611707,0.0005318052,0.0001275881,0.9500924,0.013443629,0.016745346,0.0019550768,0.003356111],"study_design_scores_gemma":[0.00012076005,0.000046548754,0.0053248913,0.000007932589,0.00001881407,0.00007989177,0.000033178752,0.9879573,0.0024619112,0.0028286611,0.0010966852,0.000023528963],"about_ca_topic_score_codex":0.0076429113,"about_ca_topic_score_gemma":0.0031172333,"teacher_disagreement_score":0.0076429113,"about_ca_system_score_codex":0.0009666295,"about_ca_system_score_gemma":0.00046506897,"threshold_uncertainty_score":0.01519686},"labels":[],"label_agreement":null},{"id":"W4319073660","doi":"10.3847/1538-4357/acac96","title":"Arp 220: A Post-starburst Galaxy with Little Current Star Formation outside of Its Nuclear Disks","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Ontario College of Art and Design","funders":"","keywords":"Physics; Astrophysics; Star formation; Astronomy; Galaxy; Star cluster; Stellar population; Population; Intergalactic star; Galaxy merger","score_opus":0.011040484039008912,"score_gpt":0.22472569722056357,"score_spread":0.21368521318155465,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319073660","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955584,0.00015783124,0.00015046018,0.00005215807,0.0000074957957,0.000003838759,0.00021844155,0.000071436385,0.0037799221],"genre_scores_gemma":[0.9983027,0.000056635494,0.00016640002,0.000047739097,0.000016292537,0.0000021383776,0.0003907262,0.000010568493,0.0010068086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999126,0.000010214106,0.000007880048,0.000028662398,0.00001912471,0.000021555317],"domain_scores_gemma":[0.999734,0.000019302586,0.00005986747,0.00003614461,0.000024842186,0.00012593904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000089754794,0.00020422571,0.00015451064,0.00047393612,0.00050166756,0.000781391,0.00036323565,0.00041504347,0.0027830575],"category_scores_gemma":[0.0002934053,0.00009577188,0.00009970416,0.00029479183,0.000306753,0.0003941324,0.00032399106,0.00023154772,0.0014433216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066948205,0.0005906091,0.84287304,0.000109254506,0.0000786452,0.0129085975,0.0019353095,0.0001623794,0.10867937,0.001478582,0.0033395472,0.027175078],"study_design_scores_gemma":[0.000014100648,0.00045759857,0.9542038,0.000017640019,0.000034210065,0.027174553,0.0011985276,0.00023483673,0.004718538,0.00029595374,0.011635094,0.000015026245],"about_ca_topic_score_codex":0.0010255313,"about_ca_topic_score_gemma":0.0011556427,"teacher_disagreement_score":0.0027830575,"about_ca_system_score_codex":0.00011669835,"about_ca_system_score_gemma":0.000049836766,"threshold_uncertainty_score":0.0093102455},"labels":[],"label_agreement":null},{"id":"W4319075150","doi":"10.3847/1538-4357/aca88f","title":"Size and Spectroscopic Evolution of HectoMAP Quiescent Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Division of Astronomical Sciences; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; U.S. Department of Energy","keywords":"Population; Redshift; Physics; Astrophysics; Galaxy; Analytical Chemistry (journal); Chemistry; Demography","score_opus":0.00611090201963554,"score_gpt":0.2151172104651688,"score_spread":0.20900630844553325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319075150","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962889,0.0001123534,0.0001258392,0.000049905895,0.0000018806342,0.0000060580724,0.0013984287,0.000053134736,0.001963454],"genre_scores_gemma":[0.997387,0.00003393564,0.00008814995,0.000023413255,0.0000055710884,0.0000053262156,0.0020550948,0.000012984522,0.00038858008],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998282,0.000023208519,0.000006943935,0.000057120968,0.000032040432,0.000052393712],"domain_scores_gemma":[0.9988564,0.00012331546,0.0004280191,0.000099886005,0.00014823873,0.0003440765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028458578,0.00020123467,0.00014597624,0.0015290129,0.0003565188,0.00086158136,0.00043161013,0.00019511243,0.0019206456],"category_scores_gemma":[0.0010528218,0.00016917524,0.00013411722,0.0010099327,0.00043828762,0.00042026042,0.00073109916,0.00020526821,0.00054952974],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018176387,0.000029452822,0.9868629,0.000017340564,0.000036584854,0.00018849167,0.00040647978,0.00025333723,0.0030060983,0.00031322436,0.002148754,0.0065555484],"study_design_scores_gemma":[0.0000038304297,0.000011676276,0.99889886,0.0000022623062,0.000004865683,0.00006428423,0.00015833242,0.00019009858,0.00013451063,0.00003273,0.0004962512,0.0000022744466],"about_ca_topic_score_codex":0.015497775,"about_ca_topic_score_gemma":0.01147573,"teacher_disagreement_score":0.015497775,"about_ca_system_score_codex":0.0005418334,"about_ca_system_score_gemma":0.00014807886,"threshold_uncertainty_score":0.030815125},"labels":[],"label_agreement":null},{"id":"W4319297600","doi":"10.3847/1538-4357/aca294","title":"Beyond UVJ: Color Selection of Galaxies in the JWST Era","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; St. Mary's University; Herzberg Institute of Astrophysics; York University","funders":"","keywords":"Physics; Galaxy; Astrophysics; Selection (genetic algorithm); Star (game theory); Astronomy; Artificial intelligence; Computer science","score_opus":0.00760003671340564,"score_gpt":0.22070093811868843,"score_spread":0.2131009014052828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319297600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96424174,0.00016576696,0.025410047,0.000071605995,0.0000150521355,0.00002740386,0.0011680266,0.0025196408,0.0063806945],"genre_scores_gemma":[0.9829842,0.000036776786,0.014186661,0.000029659337,0.000019804236,0.000008747406,0.0016071431,0.00019659165,0.00093051256],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996823,0.000060043338,0.000014469022,0.0000925024,0.00010083686,0.000049946815],"domain_scores_gemma":[0.9992478,0.00012021921,0.00014965532,0.00018486982,0.00016653643,0.00013100059],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057636254,0.00020247181,0.00030880584,0.0015307808,0.00027056658,0.0011065908,0.00036770172,0.00016124616,0.001426112],"category_scores_gemma":[0.0015440093,0.00014543162,0.0002817637,0.0010357567,0.000213612,0.00037411432,0.00063036475,0.00018256408,0.0005710996],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041048657,0.00009702078,0.6885279,0.00006304562,0.000117325086,0.00018928545,0.00040025826,0.0065341983,0.04167616,0.0019874242,0.0047964896,0.2552004],"study_design_scores_gemma":[0.000031695196,0.00009276656,0.889852,0.000017924853,0.00006725434,0.00022279279,0.00010666761,0.07506231,0.024459926,0.0013354144,0.008719862,0.000031255928],"about_ca_topic_score_codex":0.0044646524,"about_ca_topic_score_gemma":0.008298294,"teacher_disagreement_score":0.0044646524,"about_ca_system_score_codex":0.00025340077,"about_ca_system_score_gemma":0.00021334476,"threshold_uncertainty_score":0.008877337},"labels":[],"label_agreement":null},{"id":"W4319346156","doi":"10.3847/1538-4357/aca677","title":"REQUIEM-2D: A Diversity of Formation Pathways in a Sample of Spatially Resolved Massive Quiescent Galaxies at z ∼ 2","year":2023,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Grism; Astronomy; Galaxy formation and evolution; Elliptical galaxy; Hubble space telescope","score_opus":0.01866824671411966,"score_gpt":0.21499205457882217,"score_spread":0.19632380786470252,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319346156","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97734636,0.0002687337,0.0018777379,0.00010755156,0.000010934954,0.00004400042,0.015360813,0.0016348459,0.003349079],"genre_scores_gemma":[0.95037174,0.000074052296,0.005766794,0.000115165516,0.000025395972,0.000049369228,0.04151417,0.0005966677,0.0014866765],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996519,0.000054800534,0.000018254455,0.00010214895,0.000078658806,0.00009421106],"domain_scores_gemma":[0.9988362,0.00018763413,0.0001928429,0.00032966162,0.000111732545,0.00034187516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008245465,0.00049166963,0.00048629183,0.0017987088,0.00048605455,0.0010595421,0.00061037415,0.0003900576,0.0028302586],"category_scores_gemma":[0.0014760203,0.0005989624,0.0006351495,0.0010325826,0.00033875508,0.0005407984,0.0010783924,0.0003961369,0.0016173664],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013318215,0.00036679604,0.87565273,0.00016630712,0.00032469965,0.00073834416,0.0014960818,0.0063671614,0.040557172,0.0028416135,0.03736978,0.03278755],"study_design_scores_gemma":[0.000082499675,0.00006354764,0.97847086,0.000010716957,0.00003892425,0.00037315517,0.0002341568,0.0075800708,0.0037948638,0.0005868204,0.008721259,0.00004319041],"about_ca_topic_score_codex":0.0050044283,"about_ca_topic_score_gemma":0.009820254,"teacher_disagreement_score":0.0050044283,"about_ca_system_score_codex":0.00047920377,"about_ca_system_score_gemma":0.00021026006,"threshold_uncertainty_score":0.009950638},"labels":[],"label_agreement":null},{"id":"W4319346585","doi":"10.3847/1538-4357/acac99","title":"A New Physical Picture for Active Galactic Nuclei Lacking Optical Emission Lines","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Quasar; Redshift; Spectral line; Optical spectra; Emission spectrum; Galaxy; Context (archaeology); Line (geometry); Population; Astronomy; Medicine","score_opus":0.021188610964961937,"score_gpt":0.2801095217034871,"score_spread":0.25892091073852513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319346585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872902,0.00077576283,0.0053884005,0.00041791276,0.000015967898,0.000016829072,0.0003006228,0.00005384342,0.005740416],"genre_scores_gemma":[0.99835026,0.0001433007,0.00093364826,0.000072670104,0.000028390145,0.0000049301752,0.00013918364,0.0000045403526,0.00032312627],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.9998209,0.000031616797,0.000012837798,0.00007762011,0.000035590052,0.000021440645],"domain_scores_gemma":[0.99905473,0.00024312115,0.00037246005,0.00014513163,0.0000686701,0.00011592861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004336069,0.00021456527,0.00024548813,0.0012860285,0.00031954673,0.0016979598,0.0005246969,0.0004902918,0.0031695128],"category_scores_gemma":[0.0015090384,0.00012167465,0.0001726387,0.00052753196,0.0015072919,0.0020879544,0.0007646948,0.00032489395,0.00029854706],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015327815,0.00006391247,0.9458606,0.00009357453,0.000050933504,0.00064102095,0.0009374213,0.0007054665,0.024620406,0.010568599,0.00041677477,0.015887892],"study_design_scores_gemma":[0.000011839336,0.0001169039,0.9753949,0.000045398538,0.000038604823,0.00219902,0.0018167045,0.0034832493,0.0020792154,0.010640933,0.0041556736,0.000017442393],"about_ca_topic_score_codex":0.00075387675,"about_ca_topic_score_gemma":0.0009802417,"teacher_disagreement_score":0.0031695128,"about_ca_system_score_codex":0.00028193567,"about_ca_system_score_gemma":0.00013840392,"threshold_uncertainty_score":0.01060307},"labels":[],"label_agreement":null},{"id":"W4319660826","doi":"10.3847/1538-4357/ac9902","title":"Far-ultraviolet Dust Extinction and Molecular Hydrogen in the Diffuse Milky Way Interstellar Medium","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"MacEwan University","funders":"Space Telescope Science Institute","keywords":"Physics; Milky Way; Interstellar medium; Extinction (optical mineralogy); Cosmic dust; Astronomy; Astrophysics; Ultraviolet; Interstellar cloud; Astrobiology; Galaxy; Optics","score_opus":0.009837069068585459,"score_gpt":0.23081774268402433,"score_spread":0.22098067361543888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319660826","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99947554,0.00008098206,0.00005150047,0.0000044082303,6.2224234e-7,6.624607e-7,0.00010266236,0.0000051813513,0.00027842828],"genre_scores_gemma":[0.9995772,0.000041479805,0.000041398234,0.000003944877,0.0000017916293,8.6575085e-7,0.00023196354,0.0000024775418,0.00009889195],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990344,0.00001229505,0.000006111047,0.000035355333,0.000022932594,0.00001997363],"domain_scores_gemma":[0.99957913,0.000063068626,0.00018488702,0.00004874723,0.000048430564,0.000075681266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015680898,0.00018414608,0.00023713642,0.0009111167,0.00014892053,0.000655826,0.00016801506,0.00016138045,0.0007939473],"category_scores_gemma":[0.0005824052,0.00011258171,0.00020196628,0.0006821888,0.00023232437,0.00043117296,0.00059550325,0.00013163868,0.00019203166],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009106211,0.000025769747,0.9837997,0.00002460728,0.00011787447,0.000110298584,0.00016866601,0.00065457757,0.011365495,0.00009816327,0.0000896604,0.0034541315],"study_design_scores_gemma":[0.0000019819106,0.000015479543,0.99893016,0.0000029386374,0.000010139793,0.000038488277,0.000083284816,0.00018416271,0.0005476862,0.000022329352,0.0001617144,0.0000016623882],"about_ca_topic_score_codex":0.0037868335,"about_ca_topic_score_gemma":0.0072771455,"teacher_disagreement_score":0.0037868335,"about_ca_system_score_codex":0.00018553348,"about_ca_system_score_gemma":0.0000681456,"threshold_uncertainty_score":0.0075295568},"labels":[],"label_agreement":null},{"id":"W4319661314","doi":"10.3847/1538-4357/acac29","title":"GRMHD Simulations of Neutron-star Mergers with Weak Interactions: r-process Nucleosynthesis and Electromagnetic Signatures of Dynamical Ejecta","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Kilonova; Physics; Neutron star; Astrophysics; Nucleosynthesis; Ejecta; r-process; Gravitational wave; Black hole (networking); Astronomy; Stars; Supernova","score_opus":0.007765392957423011,"score_gpt":0.29755915379215886,"score_spread":0.28979376083473585,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319661314","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98993593,0.00008790248,0.0018895597,0.0002835928,0.000029894565,0.000024180168,0.0005426038,0.000110972265,0.007095438],"genre_scores_gemma":[0.99743736,0.000039430426,0.0013220827,0.000065644745,0.000012006991,0.00002346254,0.00034194737,0.0000346315,0.0007234091],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999866,0.000034282264,0.000005385264,0.00001594851,0.000027649296,0.00005068876],"domain_scores_gemma":[0.99921477,0.0003692702,0.00010987147,0.000044978722,0.00009402134,0.00016721315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041504248,0.00056541763,0.00055862154,0.00043481574,0.0007039131,0.00075898896,0.0011535491,0.0012004233,0.002109432],"category_scores_gemma":[0.0016590324,0.0004315221,0.0007915621,0.0004435885,0.00091235724,0.0003942256,0.0006777498,0.0010016036,0.00020192467],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018648649,0.000110692075,0.008584963,0.000025930607,0.00004661615,0.00016230434,0.00007825856,0.9859761,0.0013944507,0.002180303,0.00038454917,0.00086929795],"study_design_scores_gemma":[0.00004810259,0.000031234784,0.0021848213,0.00000465552,0.000008234839,0.000011641814,0.000042976262,0.9968554,0.00024787302,0.00038332317,0.00017487729,0.00000670487],"about_ca_topic_score_codex":0.035553057,"about_ca_topic_score_gemma":0.017217675,"teacher_disagreement_score":0.035553057,"about_ca_system_score_codex":0.0012932485,"about_ca_system_score_gemma":0.00091083196,"threshold_uncertainty_score":0.07069224},"labels":[],"label_agreement":null},{"id":"W4319789525","doi":"10.3847/1538-4357/acaea8","title":"The Event Horizon Telescope Image of the Quasar NRAO 530","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Canadian Institute for Advanced Research; McGill University; University of Toronto; Perimeter Institute; University of Waterloo","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; National Nuclear Security Administration; Office of Science; Directorate for Mathematical and Physical Sciences; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; National Astronomical Observatory of Japan; Universidad Nacional Autónoma de México; Recruitment Program of Global Experts; Shanghai Jiao Tong University; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Ministry of Education, India; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; European Commission; Leverhulme Trust; National Radio Astronomy Observatory; Fundação de Amparo à Pesquisa do Estado de São Paulo; Natural Sciences and Engineering Research Council of Canada; Netherlands eScience Center; European Southern Observatory; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; National Research Foundation; University of Pretoria; Compute Canada; Joint Institute for Computational Fundamental Science; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Vetenskapsrådet; U.S. Department of Energy; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Center for Theoretical Sciences; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Institutes of Natural Sciences; Government of Canada; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Flatiron Health","keywords":"Physics; Position angle; Astrophysics; Linear polarization; Polarization (electrochemistry); Quasar; Very Long Baseline Array; Brightness; Telescope; Magnetic field; Brightness temperature; Astronomy; Optics; Galaxy","score_opus":0.007056356145886876,"score_gpt":0.23161050897187052,"score_spread":0.22455415282598365,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319789525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97492313,0.00036986967,0.0022223643,0.00015603758,0.000027287724,0.000020863205,0.005385718,0.0004134326,0.016481254],"genre_scores_gemma":[0.99225944,0.00010211203,0.002304564,0.00004982536,0.000027385517,0.000004857792,0.003446441,0.000046669666,0.0017586623],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993575,0.0000029846753,0.0000015338975,0.000013986457,0.000023677594,0.000021951388],"domain_scores_gemma":[0.9998449,0.000007977582,0.000045160923,0.000019170326,0.000026670345,0.00005609808],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001739394,0.00015082433,0.00016083602,0.00070288614,0.0001809187,0.00037125516,0.0002265311,0.0001577908,0.002959031],"category_scores_gemma":[0.00014423222,0.000117389434,0.00020304987,0.00042542568,0.00012757475,0.00015270266,0.00025283435,0.00024058392,0.00061268045],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008975722,0.00021867614,0.2229819,0.00012866395,0.0001776682,0.0027138486,0.00082341436,0.001476835,0.6664885,0.0017328188,0.012082733,0.090277344],"study_design_scores_gemma":[0.000014145668,0.00007112811,0.9888959,0.000011280234,0.00002460711,0.00058517174,0.00008623475,0.001294545,0.0047816406,0.00010432287,0.004121653,0.000009345223],"about_ca_topic_score_codex":0.013466046,"about_ca_topic_score_gemma":0.021236027,"teacher_disagreement_score":0.013466046,"about_ca_system_score_codex":0.00044510365,"about_ca_system_score_gemma":0.00016622983,"threshold_uncertainty_score":0.02677536},"labels":[],"label_agreement":null},{"id":"W4319937275","doi":"10.3847/1538-4357/aca9d1","title":"Timing the r-process Enrichment of the Ultra-faint Dwarf Galaxy Reticulum II","year":2023,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"SLAC National Accelerator Laboratory; High Energy Physics; Science and Technology Facilities Council; Office of Science; Institut de Física d'Altes Energies; Conselho Nacional de Desenvolvimento Científico e Tecnológico; European Regional Development Fund; U.S. Department of Energy; European Commission; Space Telescope Science Institute; University of Portsmouth; Ohio State University; University of Illinois at Urbana-Champaign; University of Sussex; University of Pennsylvania; National Aeronautics and Space Administration; Centres de Recerca de Catalunya; Ministerio de Ciencia e Innovación; Generalitat de Catalunya; National Science Foundation","keywords":"Physics; Astrophysics; Stars; Reionization; Star formation; Dwarf galaxy; Galaxy; Astronomy; Asymptotic giant branch; Globular cluster; Redshift","score_opus":0.010579179652660637,"score_gpt":0.23169063918440289,"score_spread":0.22111145953174224,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4319937275","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9947766,0.00021175882,0.0007317132,0.00010257238,0.000011990663,0.0000058581,0.0006152729,0.00011768744,0.003426568],"genre_scores_gemma":[0.9988055,0.00002907812,0.00024237372,0.000024279789,0.000007731042,0.000002154631,0.0003749203,0.000010990039,0.00050289347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999137,0.000007935138,0.0000037209902,0.00003692711,0.000017378772,0.000020391377],"domain_scores_gemma":[0.9995697,0.00003992496,0.00014414488,0.000050354636,0.000059438564,0.00013639322],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020378943,0.00018028998,0.0001447192,0.0004285993,0.0001785125,0.0005063395,0.000254778,0.00019837287,0.0013900972],"category_scores_gemma":[0.0006516973,0.00014764222,0.00015439694,0.0002150956,0.00019249492,0.00024152137,0.00046163713,0.00022307069,0.0005020428],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039010803,0.00006200956,0.86459386,0.000091949194,0.00006952375,0.000332889,0.00035248988,0.0017431543,0.10777783,0.0031826608,0.0019700613,0.019433465],"study_design_scores_gemma":[0.0000057366356,0.000061538456,0.9913537,0.000007778919,0.000014303829,0.00010453518,0.000056092136,0.0017143531,0.0031948315,0.00028192514,0.0031976588,0.000007434151],"about_ca_topic_score_codex":0.0041613625,"about_ca_topic_score_gemma":0.0050275624,"teacher_disagreement_score":0.0041613625,"about_ca_system_score_codex":0.0006067262,"about_ca_system_score_gemma":0.00010981404,"threshold_uncertainty_score":0.008274257},"labels":[],"label_agreement":null},{"id":"W4320491261","doi":"10.3847/1538-4357/acaeb0","title":"Prospects for 21 cm Galaxy Cross-correlations with HERA and the Roman High-latitude Survey","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Physics; HERA; Astronomy; Galaxy; Astrophysics; Latitude; Particle physics","score_opus":0.012034443311209822,"score_gpt":0.24748973577549155,"score_spread":0.23545529246428173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4320491261","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9766936,0.0006391689,0.005298899,0.0010291883,0.00004283006,0.000024682526,0.001585757,0.0001873788,0.01449847],"genre_scores_gemma":[0.9966138,0.00004895075,0.0018444556,0.000071794275,0.000011955092,0.000008677638,0.0010222715,0.000020967078,0.00035704387],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9972651,0.0012741378,0.00009086194,0.00059181865,0.0004381973,0.00033994083],"domain_scores_gemma":[0.98527724,0.0045020888,0.004415518,0.0023054222,0.002367068,0.0011326186],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00825371,0.00032799804,0.00036614932,0.0012884046,0.0003097801,0.0012738415,0.00079948566,0.00053416996,0.002108024],"category_scores_gemma":[0.016726302,0.00025605233,0.00056051626,0.001330192,0.0004605545,0.001131461,0.001677114,0.0005962373,0.00058693567],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013212494,0.000020759771,0.9833181,0.000014120664,0.0000693297,0.00008601093,0.000049136434,0.004217123,0.0008313509,0.0022282184,0.00084150844,0.008192187],"study_design_scores_gemma":[0.000017118804,0.0000596243,0.9655303,0.00003129945,0.00002192991,0.0001274642,0.00012824443,0.028942259,0.0010934678,0.0010562977,0.0029641488,0.00002795225],"about_ca_topic_score_codex":0.007315659,"about_ca_topic_score_gemma":0.008389155,"teacher_disagreement_score":0.00825371,"about_ca_system_score_codex":0.0010924231,"about_ca_system_score_gemma":0.0003332578,"threshold_uncertainty_score":0.04365033},"labels":[],"label_agreement":null},{"id":"W4320730757","doi":"10.3847/1538-4357/acb139","title":"Nondetection of CHIME/Fast Radio Burst Sources with the Arecibo Observatory","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"Precursory Research for Embryonic Science and Technology; Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; McGill University; Smithsonian Astrophysical Observatory; University of Toronto; Flatiron Health; Canadian Institute for Advanced Research","keywords":"Physics; Observatory; Astronomy; Astrophysics","score_opus":0.014185028549470543,"score_gpt":0.27846883580661075,"score_spread":0.2642838072571402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4320730757","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99424547,0.0003590577,0.0025284907,0.00005421917,0.000011558325,0.000014734243,0.0004964579,0.00016642314,0.002123557],"genre_scores_gemma":[0.9969126,0.000069692,0.0016748445,0.000020884983,0.000018703795,0.000011103699,0.00093729794,0.000040748408,0.00031417728],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996012,0.000039729388,0.000020399784,0.00012307995,0.00013274614,0.00008286548],"domain_scores_gemma":[0.9968867,0.0007290467,0.001248117,0.000577722,0.0002699457,0.0002883877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00095960015,0.00034102233,0.00040552605,0.0017221582,0.0004765747,0.00071855314,0.0004677599,0.00039834314,0.0012877544],"category_scores_gemma":[0.0022852938,0.00032669387,0.00037296626,0.001010349,0.0002786158,0.00034471284,0.0006144998,0.0004279593,0.00037827838],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051607,0.000052496656,0.9291073,0.00005632021,0.00017318157,0.00045507107,0.00037859933,0.0009393844,0.045558386,0.00025966956,0.0004813899,0.022022171],"study_design_scores_gemma":[0.000009214388,0.000034766847,0.9955937,0.0000073850138,0.000021858068,0.00023642357,0.000028483402,0.0010995918,0.0020679801,0.00006686457,0.0008231318,0.000010654357],"about_ca_topic_score_codex":0.003245746,"about_ca_topic_score_gemma":0.005143294,"teacher_disagreement_score":0.003245746,"about_ca_system_score_codex":0.00044733103,"about_ca_system_score_gemma":0.00015066506,"threshold_uncertainty_score":0.006453693},"labels":[],"label_agreement":null},{"id":"W4320896688","doi":"10.3847/1538-4357/aca5fc","title":"IceCube Search for Neutrinos Coincident with Gravitational Wave Events from LIGO/Virgo Run O3","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Alberta","funders":"Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Ministry of Science and ICT, South Korea; Istituto Nazionale di Fisica Nucleare; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Academia Sinica; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Marquette University; Polarforskningssekretariatet; Ministry of Education, Culture, Sports, Science and Technology; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Centre National de la Recherche Scientifique; University of Oxford; Chiba University; Santen; Compute Canada; Vetenskapsrådet","keywords":"Physics; LIGO; Neutrino; Astrophysics; Gravitational wave; Astronomy; Neutrino detector; Neutrino astronomy; Observatory; Neutron star; Gravitational-wave observatory; Solar neutrino problem; Solar neutrino; Particle physics; Neutrino oscillation","score_opus":0.018494747243449166,"score_gpt":0.25388580938220096,"score_spread":0.2353910621387518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4320896688","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96679837,0.0004026223,0.0035304902,0.0001927904,0.00003425213,0.000088473615,0.022321165,0.0006613946,0.0059703863],"genre_scores_gemma":[0.93888164,0.00023868523,0.0091013005,0.00021779117,0.000076377415,0.00015569672,0.049723156,0.000276164,0.0013291602],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99942195,0.00011064469,0.000032820804,0.00020079732,0.00013112342,0.00010269837],"domain_scores_gemma":[0.9985475,0.00042373108,0.0005885463,0.00016122508,0.00008490691,0.00019415397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016110467,0.00047362313,0.000579483,0.0020584604,0.00063875754,0.0016558629,0.00035292565,0.0005125043,0.0032132568],"category_scores_gemma":[0.0019919921,0.0002255948,0.00068256276,0.00261857,0.00032554351,0.00027806303,0.0011387755,0.0004958253,0.00064280315],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0051910225,0.00037036175,0.8972938,0.00020533889,0.0013694124,0.001246791,0.0005375635,0.00822111,0.025942821,0.0032799563,0.021881817,0.034460023],"study_design_scores_gemma":[0.00064004713,0.00032342447,0.93786263,0.00008776263,0.00052113336,0.0006330961,0.0003245024,0.021631572,0.010893713,0.0027373524,0.0242718,0.00007308456],"about_ca_topic_score_codex":0.0062779263,"about_ca_topic_score_gemma":0.009644062,"teacher_disagreement_score":0.0062779263,"about_ca_system_score_codex":0.0004972111,"about_ca_system_score_gemma":0.00088050053,"threshold_uncertainty_score":0.012482762},"labels":[],"label_agreement":null},{"id":"W4320914686","doi":"10.3847/1538-4357/acab00","title":"Comparing the Locations of Supernovae to CO (2–1) Emission in Their Host Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"National Institutes of Natural Sciences; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; Jet Propulsion Laboratory; Ministry of Science and Technology, Taiwan; Natural Sciences and Engineering Research Council of Canada; National Science Council; Deutsche Forschungsgemeinschaft; California Institute of Technology; Canadian Institute for Theoretical Astrophysics; European Commission; Australian Government; National Radio Astronomy Observatory; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Galaxy; Milky Way; Molecular cloud; Astronomy; Interstellar medium; Star formation; Millimeter; Stars","score_opus":0.0241650534548354,"score_gpt":0.2620912660920103,"score_spread":0.23792621263717487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4320914686","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991503,0.000071253045,0.00008934168,0.0000068833474,0.0000022699912,0.0000018045727,0.00016292107,0.000007808458,0.000507397],"genre_scores_gemma":[0.9995098,0.000026677708,0.000089969035,0.0000071656855,0.0000049114137,0.0000014773526,0.00023754463,0.0000019515362,0.000120424134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998124,0.000024784831,0.000012155917,0.00006419714,0.000039848484,0.000046627378],"domain_scores_gemma":[0.99888223,0.00015520137,0.00038123777,0.00008808464,0.00015003292,0.00034313314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036220712,0.00017804893,0.00016141476,0.0014175355,0.00021334922,0.00059977995,0.00021689803,0.00026701041,0.0018632448],"category_scores_gemma":[0.00082375883,0.00015165354,0.00023204942,0.0004947105,0.00025120692,0.000288266,0.00048296686,0.00016549947,0.00032013832],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000030504925,0.000008793918,0.99544877,0.000003818474,0.000039606366,0.000021251479,0.000036861573,0.000063737694,0.0031300888,0.00003760603,0.000054623903,0.0011243345],"study_design_scores_gemma":[5.782838e-7,0.000007415832,0.99963975,8.2408104e-7,0.000004416652,0.000022459448,0.00002813663,0.000083336825,0.00014544462,0.000007284509,0.00005982182,6.173094e-7],"about_ca_topic_score_codex":0.00422621,"about_ca_topic_score_gemma":0.007928203,"teacher_disagreement_score":0.00422621,"about_ca_system_score_codex":0.00018203097,"about_ca_system_score_gemma":0.000063291394,"threshold_uncertainty_score":0.008403242},"labels":[],"label_agreement":null},{"id":"W4321116961","doi":"10.3847/1538-4357/acafec","title":"Inhomogeneous Enrichment of Radioactive Nuclei in the Galaxy: Deposition of Live <sup>53</sup>Mn, <sup>60</sup>Fe, <sup>182</sup>Hf, and <sup>244</sup>Pu into Deep-sea Archives. Surfing the Wave?","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"HORIZON EUROPE European Research Council; HORIZON EUROPE Marie Sklodowska-Curie Actions; European Cooperation in Science and Technology; U.S. Department of Energy; Science and Technology Facilities Council; National Science Foundation","keywords":"Nucleosynthesis; Physics; Galaxy; Supernova; Astrophysics; Chemical evolution; Deposition (geology); Deep sea; Astronomy; Sediment; Oceanography; Geology; Paleontology","score_opus":0.011124073291742214,"score_gpt":0.2205752154839538,"score_spread":0.2094511421922116,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116961","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987249,0.00011925353,0.0005627001,0.000025001878,0.0000013581346,0.000001155459,0.00008929692,0.000018743052,0.00045762793],"genre_scores_gemma":[0.9996147,0.000035406963,0.00015724555,0.0000048600264,7.034145e-7,6.730097e-7,0.00006312732,0.000004488159,0.000118779404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995124,0.000004959593,0.0000023133243,0.0000240225,0.0000067765295,0.000010733635],"domain_scores_gemma":[0.99979836,0.000037261234,0.00007302837,0.000024202593,0.000034505996,0.000032605254],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001656689,0.00019192549,0.00013351062,0.0004455887,0.00014523056,0.0006040674,0.00031249275,0.00030167866,0.0009997926],"category_scores_gemma":[0.00043148568,0.0001727049,0.00027722734,0.00036523453,0.00032798084,0.0003084698,0.0002495683,0.0001875056,0.00017444884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018340237,0.00002999214,0.856161,0.00003946993,0.00011229352,0.00052541454,0.00016169867,0.01945674,0.11527364,0.0013412881,0.00013980128,0.006575337],"study_design_scores_gemma":[0.000011470519,0.00006421961,0.9209939,0.0000070717847,0.00005930497,0.00032497977,0.00025455415,0.059842438,0.0169994,0.00069348456,0.0007266214,0.000022423175],"about_ca_topic_score_codex":0.013679348,"about_ca_topic_score_gemma":0.010620531,"teacher_disagreement_score":0.013679348,"about_ca_system_score_codex":0.00072280405,"about_ca_system_score_gemma":0.00014084762,"threshold_uncertainty_score":0.027199447},"labels":[],"label_agreement":null},{"id":"W4321116989","doi":"10.3847/1538-4357/acaf06","title":"Inferring the Energy and Distance Distributions of Fast Radio Bursts Using the First CHIME/FRB Catalog","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; University of Toronto; Canada Research Chairs; Canada Foundation for Innovation; National Defense Science and Engineering Graduate; Smithsonian Astrophysical Observatory; U.S. Department of Defense; U.S. Department of Energy; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Physics; Population; Algorithm; Computer science","score_opus":0.014370701870257293,"score_gpt":0.29804361764140164,"score_spread":0.28367291577114434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321116989","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8702761,0.0011282272,0.033124845,0.00032380404,0.00003472514,0.00019785968,0.07858294,0.0030083878,0.013323128],"genre_scores_gemma":[0.84330255,0.000596681,0.03532185,0.00015327001,0.000050450817,0.0001562477,0.11662323,0.00043941758,0.003356249],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995178,0.00005784742,0.00001881338,0.00014890057,0.00015862827,0.00009802665],"domain_scores_gemma":[0.99699557,0.00066478306,0.0005031271,0.0007977987,0.00066858326,0.0003701868],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011825074,0.00041604906,0.00037010212,0.004373354,0.00043634168,0.0011217447,0.0006560283,0.00043299023,0.00341612],"category_scores_gemma":[0.0049907966,0.00032526618,0.00036618527,0.0028268062,0.00017067461,0.0004522816,0.0007108262,0.00037767173,0.002426487],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022025086,0.00006370007,0.88039595,0.00009196267,0.0001399965,0.0002860434,0.00034714575,0.008111743,0.0085080005,0.0021394107,0.023237769,0.076457955],"study_design_scores_gemma":[0.000033117743,0.000022350916,0.9419086,0.000044346285,0.00004699382,0.00020850888,0.0001882819,0.022830827,0.0025438538,0.001121021,0.031012192,0.000039866405],"about_ca_topic_score_codex":0.1112226,"about_ca_topic_score_gemma":0.0954277,"teacher_disagreement_score":0.1112226,"about_ca_system_score_codex":0.001060103,"about_ca_system_score_gemma":0.0008419725,"threshold_uncertainty_score":0.2211504},"labels":[],"label_agreement":null},{"id":"W4321117797","doi":"10.3847/1538-4357/acae72","title":"Spectroscopic r-Process Abundance Retrieval for Kilonovae. I. The Inferred Abundance Pattern of Early Emission from GW170817","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto; Bishop's University; McGill University","funders":"Science and Technology Facilities Council","keywords":"Kilonova; Physics; Astrophysics; Ejecta; Nucleosynthesis; Neutron star; Stars; Supernova","score_opus":0.016693615507949365,"score_gpt":0.27432841654627804,"score_spread":0.2576348010383287,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321117797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8781401,0.00026980368,0.11107904,0.00036060638,0.000034784724,0.000038879618,0.00194307,0.004410145,0.0037237026],"genre_scores_gemma":[0.95406836,0.00005838345,0.04264881,0.00005880372,0.000015508173,0.000015704705,0.0022590298,0.0003421364,0.00053324923],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998996,0.000012404226,0.0000037291798,0.000033166256,0.000032999546,0.000018049626],"domain_scores_gemma":[0.99975413,0.00006512997,0.00005725963,0.000050725495,0.000038716804,0.000034030327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050874223,0.00052078726,0.0002897926,0.0004923088,0.00030270172,0.00049611466,0.0009668671,0.00053113943,0.0011378163],"category_scores_gemma":[0.0015793121,0.00037442797,0.0006433106,0.00033622168,0.00026372314,0.00082603877,0.0006738799,0.0006461614,0.00041120022],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015701812,0.00028595657,0.11846998,0.00032125704,0.000383546,0.0009112779,0.0005576936,0.55364686,0.20129056,0.01203714,0.005183414,0.10534221],"study_design_scores_gemma":[0.000053835156,0.000036807283,0.012157189,0.000011661504,0.000019085846,0.000098530814,0.000052348787,0.96394974,0.01917553,0.0034088364,0.0010111256,0.000025273186],"about_ca_topic_score_codex":0.004174294,"about_ca_topic_score_gemma":0.0062238663,"teacher_disagreement_score":0.004174294,"about_ca_system_score_codex":0.0004972346,"about_ca_system_score_gemma":0.0004924897,"threshold_uncertainty_score":0.008300006},"labels":[],"label_agreement":null},{"id":"W4321187695","doi":"10.3847/1538-4357/acb3be","title":"Exotic Compact Objects with Two Dark Matter Fluids","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Toronto","funders":"","keywords":"Physics; Dark matter; Dark fluid; Compact star; Astrophysics; Baryonic dark matter; Hot dark matter; Stars; Scalar field dark matter; Light dark matter; Mixed dark matter; Quark star; Astronomy; Strange matter; Dark energy; Cosmology","score_opus":0.011274890153200011,"score_gpt":0.2524946797768905,"score_spread":0.24121978962369048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321187695","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879205,0.0002075389,0.007594174,0.00004213129,0.000011344197,0.000010114171,0.000029803732,0.00004784123,0.0041365544],"genre_scores_gemma":[0.9974757,0.000031573756,0.002054531,0.000008202736,0.00001640839,0.0000046898654,0.000042729145,0.000006549366,0.00035959028],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997274,0.000055382356,0.000019999921,0.00007121409,0.00006552383,0.00006044703],"domain_scores_gemma":[0.99907625,0.00014217729,0.00034804997,0.00013650309,0.00007053594,0.00022658435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042403492,0.00049471523,0.0006275468,0.0014937716,0.0008274679,0.0022500362,0.00043557578,0.00079326483,0.0010221823],"category_scores_gemma":[0.0010374967,0.00033276255,0.0005096661,0.0005149404,0.0023043577,0.0017036411,0.0019859152,0.00037092157,0.00010581633],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061607844,0.00014012762,0.055849254,0.00028315955,0.0002495152,0.0062774466,0.0015759368,0.023283737,0.09656196,0.80151767,0.0005923966,0.013052665],"study_design_scores_gemma":[0.0003706307,0.000702661,0.1268144,0.00014862082,0.00037248922,0.021928998,0.0023365165,0.24423686,0.049720585,0.53221524,0.020861395,0.0002916308],"about_ca_topic_score_codex":0.00034327316,"about_ca_topic_score_gemma":0.00022006898,"teacher_disagreement_score":0.0022500362,"about_ca_system_score_codex":0.00046763773,"about_ca_system_score_gemma":0.00012726274,"threshold_uncertainty_score":0.003419578},"labels":[],"label_agreement":null},{"id":"W4321441535","doi":"10.3847/1538-4357/acb43f","title":"The Green Bank North Celestial Cap Survey. VII. 12 New Pulsar Timing Solutions","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Office of Naval Research; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Horizon 2020 Framework Programme; Precursory Research for Embryonic Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; European Space Agency; Canadian Institute for Advanced Research; Associated Universities; National Science Foundation","keywords":"Physics; Pulsar; Millisecond pulsar; Neutron star; Astrophysics; Green Bank Telescope; Astrometry; Astronomy; Pulsar planet; Proper motion; Gravitational wave; Fermi Gamma-ray Space Telescope; Binary pulsar; Stars","score_opus":0.04766019813851188,"score_gpt":0.32661772060567634,"score_spread":0.27895752246716443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321441535","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87664354,0.0012257441,0.002949088,0.0005149563,0.0001176049,0.00021913127,0.08768466,0.0005200284,0.030125266],"genre_scores_gemma":[0.8793795,0.0006768918,0.011315477,0.00049776066,0.00011452644,0.00022810843,0.095037945,0.00013918905,0.012610627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965787,0.000043157175,0.00003476452,0.00007324115,0.000104918996,0.00008608897],"domain_scores_gemma":[0.99875295,0.000097817676,0.00030394032,0.0001463982,0.0004212982,0.00027751413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005653595,0.00030635844,0.00019198572,0.0036935916,0.0004624715,0.0007763126,0.00033178244,0.00026858933,0.0040462897],"category_scores_gemma":[0.0011302264,0.00021042091,0.00014624988,0.0036059904,0.00015577159,0.0003167822,0.0004832784,0.00024603386,0.0016208892],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024780768,0.00003091698,0.92325985,0.000061026127,0.000049909206,0.00035447456,0.00035306026,0.00065010716,0.0034860692,0.00039113843,0.02072694,0.050388645],"study_design_scores_gemma":[0.000016942957,0.00002436793,0.9768093,0.000020836178,0.0000134828515,0.00014093469,0.00018161934,0.0008613017,0.00047120516,0.000060197315,0.021390548,0.000009130351],"about_ca_topic_score_codex":0.17989188,"about_ca_topic_score_gemma":0.37151244,"teacher_disagreement_score":0.17989188,"about_ca_system_score_codex":0.0013101146,"about_ca_system_score_gemma":0.00107981,"threshold_uncertainty_score":0.35768962},"labels":[],"label_agreement":null},{"id":"W4321441607","doi":"10.3847/1538-4357/acacff","title":"The Art of Measuring Physical Parameters in Galaxies: A Critical Assessment of Spectral Energy Distribution Fitting Techniques","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":171,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Canadian Space Agency; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Spectral energy distribution; Galaxy; Astrophysics; Distribution (mathematics); Energy distribution; Energy (signal processing); Statistical physics; Astronomy; Atomic physics","score_opus":0.012286592263916344,"score_gpt":0.2599188165442643,"score_spread":0.24763222428034795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321441607","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.11706964,0.017185122,0.8502539,0.003675568,0.00036337515,0.00021658135,0.0014901591,0.002338383,0.0074073193],"genre_scores_gemma":[0.42014122,0.007359111,0.5669407,0.0008094686,0.00045675744,0.00027159223,0.0014147959,0.0014473092,0.0011589797],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9695267,0.014878448,0.0018619471,0.0030671863,0.010312626,0.00035298083],"domain_scores_gemma":[0.83157825,0.10267134,0.011498893,0.028520882,0.02452276,0.0012078648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.050541315,0.0017824653,0.0013229204,0.008916818,0.0010902834,0.005852737,0.0033554526,0.0016027632,0.0011389365],"category_scores_gemma":[0.15271933,0.0008627677,0.0015281913,0.007890547,0.0032526797,0.005978967,0.0038566329,0.0030510575,0.0009981209],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024180337,0.0002549339,0.23076837,0.0011700778,0.0011753953,0.00012512477,0.002005126,0.09067523,0.0076203183,0.043246027,0.0066616884,0.6160559],"study_design_scores_gemma":[0.000060508562,0.00048546118,0.26769266,0.00397616,0.0003407626,0.0009834212,0.0022713162,0.47342682,0.026624328,0.14717665,0.076357834,0.00060415524],"about_ca_topic_score_codex":0.0047851107,"about_ca_topic_score_gemma":0.0023728905,"teacher_disagreement_score":0.050541315,"about_ca_system_score_codex":0.0020706456,"about_ca_system_score_gemma":0.0012005498,"threshold_uncertainty_score":0.2672912},"labels":[],"label_agreement":null},{"id":"W4321503464","doi":"10.3847/1538-4357/acac81","title":"JCMT BISTRO Observations: Magnetic Field Morphology of Bubbles Associated with NGC 6334","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of Manitoba; Western University; McMaster University; Queen's University; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec; Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; Science and Engineering Research Board; Japan Society for the Promotion of Science; National Research Foundation; Science and Technology Facilities Council; National Science and Technology Council; Ministry of Science and ICT, South Korea; Ministry of Science and Technology, Taiwan; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; National Research Foundation of Korea; European Regional Development Fund; Academia Sinica; Department of Science and Technology, Ministry of Science and Technology, India; Agencia Canaria de Investigación, Innovación y Sociedad de la Información","keywords":"Physics; Morphology (biology); Magnetic field; Astronomy; Field (mathematics); Astrophysics","score_opus":0.020788120895592184,"score_gpt":0.2277029268923359,"score_spread":0.20691480599674372,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321503464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808085,0.0000344086,0.00022389453,0.00002434566,0.0000026051778,0.0000058884534,0.00057391555,0.0000821229,0.0009719536],"genre_scores_gemma":[0.99861896,0.000014411322,0.0004261633,0.000010995806,0.0000050988965,0.0000033750857,0.0007121703,0.000010687852,0.00019813879],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999528,0.0000030267397,0.0000019690224,0.000011891633,0.000017236003,0.000013001921],"domain_scores_gemma":[0.9997311,0.000027931592,0.00007971599,0.000024143012,0.000058742684,0.00007829411],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007900021,0.00012937828,0.00011370461,0.00136954,0.00024922134,0.00023188643,0.00019179012,0.00024991066,0.0011631398],"category_scores_gemma":[0.00031299784,0.00007991772,0.00007439139,0.0006239928,0.0001245127,0.00016919394,0.00024015832,0.00016864824,0.00017334882],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025461247,0.00008772679,0.7490844,0.000040159655,0.000045588422,0.001112838,0.00054316735,0.0011590868,0.22303109,0.00023229737,0.0023414176,0.022067677],"study_design_scores_gemma":[0.000004259522,0.000016672617,0.996157,0.0000025058116,0.0000059044796,0.00013166698,0.00007646683,0.0013992507,0.0017592832,0.000026707101,0.00041624164,0.0000041341755],"about_ca_topic_score_codex":0.010839794,"about_ca_topic_score_gemma":0.024386048,"teacher_disagreement_score":0.010839794,"about_ca_system_score_codex":0.00021040063,"about_ca_system_score_gemma":0.00007437465,"threshold_uncertainty_score":0.021553397},"labels":[],"label_agreement":null},{"id":"W4321503650","doi":"10.3847/1538-4357/acb13d","title":"A Multiwavelength Study of Active Galactic Nuclei in Post-merger Remnants","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Active galactic nucleus; Astrophysics; Galaxy; Sky; Luminosity; Redshift; Stellar mass; Astronomy; Star formation","score_opus":0.011465059929046372,"score_gpt":0.24239304791317537,"score_spread":0.230927987984129,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321503650","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99972206,0.0000847856,0.00004028401,0.0000041570547,3.9714791e-7,0.0000014176588,0.000022701846,0.0000013411441,0.00012282278],"genre_scores_gemma":[0.9997136,0.000035387915,0.000059958755,0.000004826299,0.0000023574432,9.1279725e-7,0.000060451322,8.9516436e-7,0.00012161807],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998841,0.000019768995,0.0000083432715,0.0000280973,0.000029947212,0.000029728786],"domain_scores_gemma":[0.9993217,0.00010832005,0.00032697938,0.000041270083,0.00006884375,0.00013284174],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028823328,0.00012470318,0.00019997456,0.00085223163,0.00025585783,0.00039533878,0.00018364706,0.00016647267,0.0007881412],"category_scores_gemma":[0.0005857389,0.00009472926,0.00016069345,0.00033682963,0.00022299074,0.00020062352,0.00031947854,0.00012995348,0.00019023403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014364537,0.000053109878,0.9699783,0.00001066489,0.00003935005,0.0003776441,0.00031506547,0.000075018885,0.026290363,0.000044804583,0.000023958071,0.0026480816],"study_design_scores_gemma":[0.0000010514539,0.000052431325,0.998769,0.0000012259609,0.000006935567,0.00025311962,0.00012620732,0.000076028125,0.0006241272,0.000009797605,0.00007919492,8.8864357e-7],"about_ca_topic_score_codex":0.0025855214,"about_ca_topic_score_gemma":0.0032047962,"teacher_disagreement_score":0.0025855214,"about_ca_system_score_codex":0.00015440371,"about_ca_system_score_gemma":0.00008492912,"threshold_uncertainty_score":0.00514096},"labels":[],"label_agreement":null},{"id":"W4321503936","doi":"10.3847/1538-4357/ac9400","title":"GALFIT-ing AGN Host Galaxies in COSMOS: HST versus Subaru","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Subaru Telescope; Astrophysics; Galaxy; Astronomy; Active galactic nucleus; Redshift; Hubble Deep Field; RADIUS; Spectral line; Spectrograph","score_opus":0.014011929721795675,"score_gpt":0.2345565779675344,"score_spread":0.22054464824573872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321503936","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9826245,0.00017216128,0.005008818,0.00010815745,0.000024148821,0.000014875161,0.0042392975,0.0038084732,0.0039995923],"genre_scores_gemma":[0.98268545,0.00006609307,0.004906351,0.00007473993,0.000023674449,0.000020826104,0.010456082,0.0010816144,0.000685153],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954695,0.00014106224,0.000022935987,0.00012596424,0.00010716312,0.00005594984],"domain_scores_gemma":[0.99800164,0.0008548893,0.00029849794,0.00041682096,0.00019945137,0.00022881023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015896064,0.00056065625,0.0004527347,0.0021306805,0.00027353148,0.001302421,0.0005565908,0.00034782846,0.00351134],"category_scores_gemma":[0.004156289,0.0001706066,0.00071353413,0.0019990716,0.00033312978,0.0005485527,0.0009445173,0.00047322505,0.0019110835],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079936,0.00026691557,0.8287528,0.00013548466,0.00075830636,0.00043353083,0.0005237024,0.09801373,0.00751811,0.0025687262,0.01662514,0.04360418],"study_design_scores_gemma":[0.00006620166,0.0001499157,0.6860148,0.00003221013,0.00009459745,0.000342565,0.00067809125,0.29803517,0.0056499247,0.0016784831,0.007198188,0.00005972967],"about_ca_topic_score_codex":0.0032090794,"about_ca_topic_score_gemma":0.0030263297,"teacher_disagreement_score":0.00351134,"about_ca_system_score_codex":0.00034336577,"about_ca_system_score_gemma":0.00016778451,"threshold_uncertainty_score":0.011746585},"labels":[],"label_agreement":null},{"id":"W4321602567","doi":"10.3847/1538-4357/acaf71","title":"MOMO. VI. Multifrequency Radio Variability of the Blazar OJ 287 from 2015 to 2022, Absence of Predicted 2021 Precursor-flare Activity, and a New Binary Interpretation of the 2016/2017 Outburst","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Flare; Blazar; Astrophysics; Binary number; Astronomy; Gamma ray","score_opus":0.009617272792782912,"score_gpt":0.2396722791322672,"score_spread":0.2300550063394843,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4321602567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976472,0.00004386205,0.00009123207,0.000026402011,0.0000046713644,0.0000041523654,0.0009825205,0.000014628947,0.001185272],"genre_scores_gemma":[0.99819094,0.000016130749,0.00008612413,0.00000892659,0.0000064969895,0.0000019908894,0.0014221112,0.000003863487,0.00026338504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999548,0.0000020021484,0.000002230946,0.000012307155,0.000011300964,0.00001733415],"domain_scores_gemma":[0.99973696,0.000017456106,0.000114155664,0.000016678177,0.00003734817,0.00007743165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013903169,0.00014500598,0.000119767144,0.0005323384,0.00022976528,0.00047894646,0.00013318956,0.00013552117,0.0008813042],"category_scores_gemma":[0.0002916772,0.00006296727,0.00011599873,0.00029487585,0.00015108082,0.00012837833,0.00031740076,0.00023756755,0.0002676601],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030169543,0.00006486243,0.9708429,0.000031158663,0.00002851701,0.00041184173,0.00026982155,0.00044908503,0.018509034,0.00024662912,0.0007951713,0.00804934],"study_design_scores_gemma":[0.0000023780863,0.000016914948,0.9985158,0.0000032189132,0.0000067624146,0.000065265725,0.00007267023,0.0003410703,0.0005209823,0.000021025691,0.00043209878,0.0000017688067],"about_ca_topic_score_codex":0.009319187,"about_ca_topic_score_gemma":0.018834807,"teacher_disagreement_score":0.009319187,"about_ca_system_score_codex":0.00031822702,"about_ca_system_score_gemma":0.0001673528,"threshold_uncertainty_score":0.018529892},"labels":[],"label_agreement":null},{"id":"W4322494044","doi":"10.3847/1538-4357/acb057","title":"Using Host Galaxy Photometric Redshifts to Improve Cosmological Constraints with Type Ia Supernovae in the LSST Era","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canada Research Chairs; University of Toronto","funders":"Centre National de la Recherche Scientifique; U.S. Department of Energy; Science and Technology Facilities Council; Institut National de Physique Nucléaire et de Physique des Particules; Office of Science; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Dark energy; Photometric redshift; Cosmology; Galaxy; Large Synoptic Survey Telescope; Cosmic microwave background; Supernova; Light curve; Luminosity; Astronomy","score_opus":0.028124473886797896,"score_gpt":0.28118787166266224,"score_spread":0.25306339777586434,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322494044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9875228,0.000100239864,0.010357254,0.00009013302,0.000007676804,0.000010501857,0.0008672635,0.0002510021,0.00079304166],"genre_scores_gemma":[0.99036646,0.000034595723,0.006776059,0.000042718788,0.0000159939,0.000007594194,0.0025594514,0.00005418774,0.00014294144],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999185,0.0003974189,0.00004887541,0.00017034078,0.000133406,0.00006495621],"domain_scores_gemma":[0.99267465,0.003438864,0.0011164836,0.0015737293,0.0008037765,0.00039249656],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0045555104,0.0005665743,0.0005832143,0.0009068846,0.0003325342,0.0012448308,0.0007941365,0.0004517064,0.001114165],"category_scores_gemma":[0.013153697,0.00035267288,0.0008528807,0.00090875285,0.00041204898,0.0012101174,0.0012043077,0.0004938363,0.0002616008],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000470387,0.00015557212,0.6177761,0.00006212801,0.000549579,0.000077792625,0.00006845725,0.35583067,0.0038719135,0.001874663,0.0010646005,0.018198151],"study_design_scores_gemma":[0.000079438076,0.00015320884,0.1864813,0.00002209278,0.000109528504,0.000052171043,0.00004579084,0.8067229,0.0028055024,0.002232242,0.001268479,0.00002734713],"about_ca_topic_score_codex":0.011500162,"about_ca_topic_score_gemma":0.015614848,"teacher_disagreement_score":0.011500162,"about_ca_system_score_codex":0.0005113846,"about_ca_system_score_gemma":0.0007111697,"threshold_uncertainty_score":0.024092138},"labels":[],"label_agreement":null},{"id":"W4322494050","doi":"10.3847/1538-4357/acb0c5","title":"Early-forming Massive Stars Suppress Star Formation and Hierarchical Cluster Assembly","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Supercomputing Center, Korea Institute of Science and Technology Information; Natural Sciences and Engineering Research Council of Canada; Universität Heidelberg; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Deutsche Forschungsgemeinschaft; Leibniz-Gemeinschaft; National Aeronautics and Space Administration; New York Space Grant Consortium; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Stars; Star cluster; Cluster (spacecraft); Star (game theory); Astronomy","score_opus":0.012239284166457821,"score_gpt":0.24653824436837235,"score_spread":0.23429896020191454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322494050","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99783283,0.000015666965,0.0014532002,0.000014732188,0.000003397518,0.000004710212,0.00004097902,0.00016487557,0.0004696086],"genre_scores_gemma":[0.99908555,0.000008384654,0.00068500487,0.000007822128,0.0000011356901,0.000004041479,0.000039328697,0.000019270063,0.00014935629],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998098,0.000054564487,0.000007644719,0.00003585511,0.00005029804,0.00004187416],"domain_scores_gemma":[0.9991756,0.000275199,0.00020677231,0.00010721325,0.00006736039,0.00016774292],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030134522,0.0003180523,0.00032074412,0.00023961214,0.0002682229,0.00060637615,0.0006027153,0.00025601254,0.0010894166],"category_scores_gemma":[0.0014919335,0.00019438379,0.00024995144,0.00011896708,0.00064594497,0.00027893262,0.0006960184,0.00028236932,0.00012618498],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015477424,0.000872276,0.08715139,0.00019327133,0.00018378434,0.00025511745,0.00022548222,0.5987222,0.28603023,0.008297147,0.001680408,0.014840952],"study_design_scores_gemma":[0.00021246892,0.00068496255,0.037311193,0.000008062407,0.00005721567,0.00006430722,0.00006919057,0.87708163,0.080239,0.0031255325,0.001116331,0.000030092511],"about_ca_topic_score_codex":0.0042354227,"about_ca_topic_score_gemma":0.003287966,"teacher_disagreement_score":0.0042354227,"about_ca_system_score_codex":0.00053834805,"about_ca_system_score_gemma":0.00043451865,"threshold_uncertainty_score":0.00842154},"labels":[],"label_agreement":null},{"id":"W4322494096","doi":"10.3847/1538-4357/acb6ff","title":"Simple Physics and Integrators Accurately Reproduce Mercury Instability Statistics","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Instability; Solar System; Planet; Exoplanet; Astrophysics; Statistical physics; Astronomy; Quantum mechanics","score_opus":0.027176782967871314,"score_gpt":0.2751560641694973,"score_spread":0.24797928120162596,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322494096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8938407,0.00021590968,0.09436408,0.00043575894,0.00014632354,0.00009299028,0.0012652986,0.0018719574,0.0077670915],"genre_scores_gemma":[0.978834,0.00005942614,0.01940748,0.00006803826,0.000028124781,0.00006554542,0.0007562183,0.00020894474,0.0005722546],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99969673,0.00007846708,0.000025749267,0.00006584856,0.00008089244,0.00005236135],"domain_scores_gemma":[0.99789774,0.00092017074,0.00022221777,0.000484987,0.00032749426,0.00014736131],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012254157,0.00054684695,0.00088580576,0.00080382585,0.0008626982,0.0009165686,0.0013448552,0.0009252928,0.0020535558],"category_scores_gemma":[0.007511424,0.00039384564,0.0008682015,0.00054190727,0.0007364131,0.0013174603,0.0006671631,0.0010922087,0.00035065916],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004005365,0.00007600543,0.0088765295,0.000048770933,0.0000716179,0.00007883982,0.000068447596,0.9762215,0.0016178415,0.0070194625,0.0010232849,0.004857693],"study_design_scores_gemma":[0.0000128040165,0.000013423063,0.000985223,0.0000041964877,0.000007257854,0.0000075502,0.000008288066,0.9959031,0.00036298705,0.0024430265,0.00024436382,0.000007843578],"about_ca_topic_score_codex":0.017174793,"about_ca_topic_score_gemma":0.01334304,"teacher_disagreement_score":0.017174793,"about_ca_system_score_codex":0.00092225045,"about_ca_system_score_gemma":0.001466605,"threshold_uncertainty_score":0.034149647},"labels":[],"label_agreement":null},{"id":"W4322494175","doi":"10.3847/1538-4357/acae96","title":"A Large-scale Kinematic Study of Molecular Gas in High-z Cluster Galaxies: Evidence for High Levels of Kinematic Asymmetry","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto; York University","funders":"National Astronomical Observatory of Japan; National Radio Astronomy Observatory; Arizona State University; National Institutes of Natural Sciences; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Asymmetry; Redshift; Astronomy; Kinematics; Galaxy rotation curve; Galaxy formation and evolution; Galaxy cluster; Classical mechanics","score_opus":0.018992187268974,"score_gpt":0.26780782790391683,"score_spread":0.24881564063494283,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322494175","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995109,0.00002143606,0.00014609518,0.000006577014,3.7850447e-7,0.0000014643259,0.00007095376,0.000006997991,0.00023524494],"genre_scores_gemma":[0.9998369,0.0000064630044,0.000054111853,0.0000020904806,9.536187e-7,6.7320235e-7,0.00007224618,0.0000011695284,0.000025385212],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998204,0.000020049296,0.000008280888,0.000058393238,0.00004490755,0.00004797716],"domain_scores_gemma":[0.9991697,0.00013312779,0.00030654523,0.00011322463,0.00011402704,0.00016333353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000298823,0.00018135652,0.00026949175,0.0013197026,0.00041585736,0.00063208933,0.00036938267,0.00021678349,0.0008750958],"category_scores_gemma":[0.00079396245,0.00015576163,0.000243215,0.0010157281,0.00058740604,0.0003388011,0.0005955538,0.00016919298,0.00019050666],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004968783,0.000014149393,0.99074054,0.000005070063,0.000038425263,0.000035396348,0.00018889354,0.00036667922,0.006953632,0.00014689565,0.00003380195,0.0014268464],"study_design_scores_gemma":[9.524518e-7,0.000008683201,0.99933845,5.808029e-7,0.0000039280303,0.000017427777,0.000053952583,0.00030687024,0.00021245824,0.00002492717,0.000030491175,0.0000013274617],"about_ca_topic_score_codex":0.008683068,"about_ca_topic_score_gemma":0.007164016,"teacher_disagreement_score":0.008683068,"about_ca_system_score_codex":0.0003505071,"about_ca_system_score_gemma":0.00016724959,"threshold_uncertainty_score":0.017265022},"labels":[],"label_agreement":null},{"id":"W4322628186","doi":"10.3847/1538-4357/acb693","title":"Does Turbulence along the Coronal Current Sheet Drive Ion Cyclotron Waves?","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council; Goddard Space Flight Center; Bundesministerium für Wirtschaft und Energie; Agenzia Spaziale Italiana; Office of Experimental Program to Stimulate Competitive Research; National Science Foundation; Swedish National Space Agency; Istituto Nazionale di Astrofisica; National Aeronautics and Space Administration","keywords":"Physics; Current sheet; Cyclotron; Turbulence; Current (fluid); Astrophysics; Astronomy; Ion; Computational physics; Atomic physics; Nuclear physics; Magnetohydrodynamics; Plasma; Mechanics","score_opus":0.008365855423097836,"score_gpt":0.24441860857586845,"score_spread":0.2360527531527706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322628186","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99565965,0.00047544262,0.0016182363,0.00019903382,0.000023927409,0.0000069367807,0.000059436647,0.000035844078,0.0019214401],"genre_scores_gemma":[0.9996836,0.00011126693,0.000087422406,0.000009394107,0.000010889127,7.686366e-7,0.000017523476,0.000001012028,0.00007814695],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999714,0.0000034590605,0.00000206006,0.000007829199,0.0000051737525,0.000010177667],"domain_scores_gemma":[0.99981374,0.00004676906,0.00007682692,0.000021005453,0.000021607952,0.000020054096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012600559,0.00010062626,0.00013664828,0.000207059,0.00012464255,0.0005647649,0.00012907332,0.00023235162,0.0005730554],"category_scores_gemma":[0.00039347616,0.000085298736,0.00008370164,0.00015441947,0.0003531055,0.00036105028,0.00012003651,0.00014591696,0.00013310894],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082790264,0.0001308933,0.44461712,0.0002164441,0.00009831432,0.0024902197,0.0007052917,0.0038414218,0.4975975,0.010582877,0.000997168,0.03789481],"study_design_scores_gemma":[0.00005647033,0.0002768641,0.88999575,0.000043133485,0.000049868646,0.0011078551,0.0011030483,0.038406543,0.056043588,0.009974662,0.0029104885,0.000031649444],"about_ca_topic_score_codex":0.0006381472,"about_ca_topic_score_gemma":0.0003091779,"teacher_disagreement_score":0.0006381472,"about_ca_system_score_codex":0.0001198326,"about_ca_system_score_gemma":0.00006167489,"threshold_uncertainty_score":0.0019171238},"labels":[],"label_agreement":null},{"id":"W4322628235","doi":"10.3847/1538-4357/acb8bc","title":"Structure and Kinematics of Sh2-138—A Distant Hub-filament System in the Outer Galactic Plane","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Protein filament; Astrophysics; Galactic plane; Line (geometry); Supersonic speed; Spectral line; Position (finance); Molecular cloud; Telescope; Galactic Center; Astronomy; Galaxy; Geometry; Stars","score_opus":0.009877851029873354,"score_gpt":0.2329283979308394,"score_spread":0.22305054690096604,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322628235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938035,0.000013572949,0.000037653444,0.000003817751,3.8432248e-7,0.0000023771463,0.00007796434,0.0000051348857,0.0004787557],"genre_scores_gemma":[0.99943,0.000009062251,0.00010788886,0.0000020479586,0.000001279245,0.0000011646238,0.00026249705,0.0000014429057,0.00018458039],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999502,0.0000037874977,0.00000181348,0.000013421072,0.000014368407,0.000016458527],"domain_scores_gemma":[0.9998888,0.0000030771107,0.000029472434,0.0000061141404,0.000018321469,0.000054276898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005144295,0.00015126476,0.00015171501,0.00055869954,0.00035822144,0.00035927087,0.00024180616,0.00012960797,0.0012181881],"category_scores_gemma":[0.00011035012,0.00006981329,0.00010214613,0.00058343,0.000182388,0.00013905794,0.0004272651,0.00008723573,0.00028195718],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018821261,0.00007337823,0.950307,0.000013410775,0.000028940736,0.00067722856,0.00061442755,0.00061506376,0.04022926,0.0003419384,0.00032665912,0.006584335],"study_design_scores_gemma":[0.0000063953853,0.00005306885,0.9970788,0.000001941411,0.000005755899,0.00020720287,0.00027716497,0.0010109011,0.00073705654,0.00004877489,0.000570158,0.000002790539],"about_ca_topic_score_codex":0.02167399,"about_ca_topic_score_gemma":0.019416228,"teacher_disagreement_score":0.02167399,"about_ca_system_score_codex":0.00045075815,"about_ca_system_score_gemma":0.00016300818,"threshold_uncertainty_score":0.04309565},"labels":[],"label_agreement":null},{"id":"W4322734788","doi":"10.3847/1538-4357/acb3b2","title":"CO Excitation in High-z Main-sequence Analogues: Resolved CO(4−3)/CO(3−2) Line Ratios in DYNAMO Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Institutes of Natural Sciences; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; Universidad de Concepción; Universities Space Research Association; Australian Government; Universität Stuttgart; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Max-Planck-Gesellschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Dynamo; Star formation; Line (geometry); Carbon monoxide; Astronomy; Magnetic field","score_opus":0.016837797516694116,"score_gpt":0.2596018643281792,"score_spread":0.2427640668114851,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4322734788","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994042,0.000030131403,0.000088005356,0.000005900193,5.9950764e-7,0.000001496509,0.00012247068,0.000009463081,0.0003377289],"genre_scores_gemma":[0.99964774,0.0000088933675,0.000066616354,0.0000055358855,0.0000010876308,0.0000013094921,0.00014639192,0.0000032003456,0.00011927065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995315,0.0000035311107,0.0000020321543,0.000020330897,0.000008480724,0.00001254317],"domain_scores_gemma":[0.99972445,0.000028402448,0.000095140604,0.000022118626,0.000036133722,0.00009375888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011248138,0.00011902653,0.00014040137,0.00074412255,0.00017328504,0.00036640422,0.0001501157,0.0001710335,0.0011556504],"category_scores_gemma":[0.00029555472,0.00012333482,0.00010475264,0.0003449127,0.00017723218,0.00015964608,0.00024940248,0.00012569394,0.00029269257],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000212465,0.000042573516,0.94521254,0.000010061009,0.000031896427,0.00008085123,0.00019228838,0.00024881854,0.049896833,0.00007192476,0.0001578814,0.0038418197],"study_design_scores_gemma":[0.0000011117394,0.00000863058,0.99887186,5.9411735e-7,0.0000027047242,0.000022067265,0.00003177138,0.00021931702,0.00076364324,0.000010947481,0.00006648325,9.1825746e-7],"about_ca_topic_score_codex":0.0044231256,"about_ca_topic_score_gemma":0.0064544072,"teacher_disagreement_score":0.0044231256,"about_ca_system_score_codex":0.00027034176,"about_ca_system_score_gemma":0.000048709706,"threshold_uncertainty_score":0.008794725},"labels":[],"label_agreement":null},{"id":"W4323031646","doi":"10.3847/1538-4357/acac27","title":"SOFIA and ALMA Investigate Magnetic Fields and Gas Structures in Massive Star Formation: The Case of the Masquerading Monster in BYF 73","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Universities Space Research Association","keywords":"Physics; Monster; Astrophysics; Astronomy; Star formation; Star (game theory); Magnetic field; Stars","score_opus":0.011066042041915672,"score_gpt":0.22859097041208515,"score_spread":0.21752492837016948,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323031646","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987048,0.000023446448,0.00001622947,0.000058180744,0.0000013790142,0.0000012451454,0.00006437314,0.0000019530128,0.001128406],"genre_scores_gemma":[0.99974364,0.000012227211,0.00002753561,0.00000957748,0.000001941435,4.969022e-7,0.000052646512,8.119752e-7,0.00015113811],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999211,0.000008482896,0.0000013788672,0.000011238826,0.000010702584,0.000046985908],"domain_scores_gemma":[0.99986196,0.000014459262,0.000030714004,0.000010331993,0.000016548198,0.00006592492],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013408078,0.00008639462,0.00012932021,0.0006583021,0.0007918401,0.00055068743,0.00019618694,0.00020699462,0.000985548],"category_scores_gemma":[0.00022374657,0.000049047685,0.00008413063,0.0005028994,0.00047980598,0.000257821,0.00042723824,0.00023290857,0.00010634193],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014318604,0.000035857534,0.983052,0.000008224644,0.000021370019,0.0017914831,0.0024168766,0.00024446362,0.003994559,0.0006247525,0.00079097436,0.0068761106],"study_design_scores_gemma":[0.000002509898,0.000014061962,0.9959001,0.0000033576732,0.000004520549,0.00013325216,0.002264563,0.00033329864,0.00019257348,0.0000598556,0.0010897844,0.0000022011698],"about_ca_topic_score_codex":0.1537095,"about_ca_topic_score_gemma":0.224319,"teacher_disagreement_score":0.1537095,"about_ca_system_score_codex":0.0014022447,"about_ca_system_score_gemma":0.00046620768,"threshold_uncertainty_score":0.3056296},"labels":[],"label_agreement":null},{"id":"W4323319278","doi":"10.3847/1538-4357/acb352","title":"Does the HCN/CO Ratio Trace the Star-forming Fraction of Gas? I. A Comparison with Analytical Models of Star Formation","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Institutes of Natural Sciences; Canada Research Chairs; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Star formation; Galaxy; Stellar mass; Star (game theory); Power law; Context (archaeology); Statistics","score_opus":0.0230423890678102,"score_gpt":0.27680374495566007,"score_spread":0.25376135588784987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323319278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9647948,0.00074898754,0.028830834,0.00029439857,0.000020610598,0.000024320054,0.000356811,0.00020790512,0.004721387],"genre_scores_gemma":[0.9981439,0.000087582775,0.0015150796,0.000016213395,0.000008458078,0.0000052133014,0.000068411624,0.000012839705,0.00014234701],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995172,0.0001572545,0.000025545149,0.00013874723,0.00011431968,0.000047035195],"domain_scores_gemma":[0.99683183,0.0015725885,0.00058080803,0.0006310543,0.00025792207,0.00012576905],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016269083,0.00038150587,0.00029250956,0.0012177015,0.00020262304,0.0014428028,0.00143504,0.0006071239,0.0008529657],"category_scores_gemma":[0.0078076324,0.00019946041,0.0004932377,0.0009506901,0.0008782818,0.00143836,0.00047556864,0.00033722646,0.00028783348],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005607561,0.00019892523,0.6214204,0.00015870246,0.00035686456,0.00014991511,0.00032278252,0.31870213,0.0073667653,0.024045171,0.0007801704,0.025937343],"study_design_scores_gemma":[0.000021507547,0.00012430751,0.16899636,0.000025796653,0.00004286687,0.00015686196,0.00022961939,0.8148121,0.0024207106,0.012365378,0.0007710884,0.000033384433],"about_ca_topic_score_codex":0.010954678,"about_ca_topic_score_gemma":0.006000546,"teacher_disagreement_score":0.010954678,"about_ca_system_score_codex":0.0014344122,"about_ca_system_score_gemma":0.0004455426,"threshold_uncertainty_score":0.021781802},"labels":[],"label_agreement":null},{"id":"W4323354969","doi":"10.3847/1538-4357/acb92d","title":"A Complex Dust Morphology in the High-luminosity AGN Mrk 876","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; National Research Foundation","keywords":"Physics; Astrophysics; Accretion (finance); Active galactic nucleus; Black-body radiation; Astronomy; RADIUS; Luminosity; Emissivity; Wavelength; Cosmic dust; Galaxy; Radiation","score_opus":0.01814696729790817,"score_gpt":0.23546812635910405,"score_spread":0.21732115906119587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323354969","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986871,0.000073537216,0.00031936195,0.000008859616,0.0000013584394,0.0000014481946,0.000102393904,0.000019378658,0.00078656554],"genre_scores_gemma":[0.9995012,0.0000127834155,0.0001818534,0.0000059823196,0.000003190966,6.0220185e-7,0.00010696587,0.000004724914,0.00018267785],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999397,0.0000047887315,0.0000035664293,0.000019777599,0.000019412646,0.000012746115],"domain_scores_gemma":[0.99979407,0.00003074222,0.00008532806,0.000022570648,0.000031400497,0.000035944522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009311405,0.00011840156,0.0001831693,0.00047928604,0.00017871073,0.0004096821,0.00016596787,0.00016867978,0.00093683606],"category_scores_gemma":[0.00015948464,0.00009306266,0.00010597164,0.0002659928,0.0001976132,0.00010366948,0.00021174944,0.00015422699,0.0003102187],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027721762,0.000077071796,0.58697426,0.000052627714,0.00004934623,0.0012447176,0.00026578995,0.0010476342,0.39804235,0.00030937413,0.0003163613,0.011343328],"study_design_scores_gemma":[0.0000021693158,0.000025625677,0.9941691,0.0000012596546,0.0000056311255,0.0007508794,0.000035437304,0.0005184194,0.0041914494,0.000045000936,0.00025270612,0.0000024608332],"about_ca_topic_score_codex":0.0008688838,"about_ca_topic_score_gemma":0.0008389477,"teacher_disagreement_score":0.00093683606,"about_ca_system_score_codex":0.00012416259,"about_ca_system_score_gemma":0.00003345519,"threshold_uncertainty_score":0.0031340122},"labels":[],"label_agreement":null},{"id":"W4323354972","doi":"10.3847/1538-4357/acb496","title":"X-Ray Polarimetry Reveals the Magnetic-field Topology on Sub-parsec Scales in Tycho’s Supernova Remnant","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Nationaal Regieorgaan Onderwijsonderzoek; Horizon 2020 Framework Programme; Marshall Space Flight Center; National Natural Science Foundation of China; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Goddard Space Flight Center; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Hong Kong Government; Istituto Nazionale di Fisica Nucleare; European Commission; China National Funds for Distinguished Young Scientists; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Supernova remnant; Magnetic field; Particle acceleration; Polarization (electrochemistry); Synchrotron; Supernova; Degree of polarization; Astronomy; Optics; Scattering","score_opus":0.011223476052475501,"score_gpt":0.2427038912779503,"score_spread":0.2314804152254748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323354972","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99921584,0.0000287545,0.00016272538,0.0000063038765,7.648702e-7,0.0000015082985,0.00012659043,0.000016159605,0.000441274],"genre_scores_gemma":[0.99932146,0.000026719757,0.00017180815,0.0000045155684,0.0000027346446,0.0000025306817,0.00030843704,0.000006942276,0.0001548851],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997175,0.000001868198,0.0000015733094,0.000009629494,0.000005844266,0.0000093496],"domain_scores_gemma":[0.99986994,0.000013847181,0.00004977035,0.000016821452,0.000020629897,0.000028898368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000063399704,0.00015760268,0.00012159439,0.0006724836,0.0001598508,0.0004702104,0.000118454394,0.00011506595,0.0010109483],"category_scores_gemma":[0.00017051894,0.0001307627,0.00012529151,0.00030680562,0.00019549063,0.00013363085,0.00034564344,0.00017698426,0.00020434726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046747382,0.000029984492,0.50314194,0.000034599667,0.00008225955,0.00078467047,0.00043021457,0.0010540358,0.48672032,0.00030858023,0.00019220368,0.0067536277],"study_design_scores_gemma":[0.0000039435845,0.000014496345,0.9948426,0.0000019502843,0.000008335219,0.00014475753,0.000101998376,0.0006762499,0.003983151,0.00003835441,0.00018143232,0.0000027492956],"about_ca_topic_score_codex":0.0030504037,"about_ca_topic_score_gemma":0.002000144,"teacher_disagreement_score":0.0030504037,"about_ca_system_score_codex":0.000110234534,"about_ca_system_score_gemma":0.000061080515,"threshold_uncertainty_score":0.006065309},"labels":[],"label_agreement":null},{"id":"W4323544118","doi":"10.3847/1538-4357/acb1b0","title":"X-Ray Studies of the Pulsar PSR J1420–6048 and Its TeV Pulsar Wind Nebula in the Kookaburra Region","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Pulsar wind nebula; Pulsar; Millisecond pulsar; Astronomy; Spectral energy distribution; Spectral index; Nebula; Torus; Spectral line; Stars; Galaxy","score_opus":0.03859822445462389,"score_gpt":0.3515985487088179,"score_spread":0.313000324254194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323544118","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995478,0.00008225371,0.000047510053,0.0000031717998,6.207545e-7,0.0000019876234,0.0000475905,0.0000036424005,0.000265519],"genre_scores_gemma":[0.9991159,0.00011329143,0.00020911559,0.000008383334,0.00000466146,0.000005430013,0.00029606544,0.0000048583424,0.00024222163],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999224,0.0000060464895,0.0000066025773,0.000022662976,0.000023146798,0.000019207257],"domain_scores_gemma":[0.9997851,0.000019065657,0.000088555425,0.000020603848,0.000029234385,0.000057422676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012731917,0.00021002801,0.00028908395,0.0013125964,0.00045071307,0.0003322503,0.000221665,0.000194475,0.00065757876],"category_scores_gemma":[0.00023730178,0.00016776676,0.00017306955,0.0007313281,0.00018337043,0.00024918548,0.0005111758,0.00014904441,0.00019008551],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003354484,0.00013695538,0.7424927,0.00007840937,0.00009943467,0.0018564695,0.0008514448,0.00055694644,0.23857465,0.00019516045,0.00018886724,0.014633473],"study_design_scores_gemma":[0.000004480595,0.00006912327,0.9968382,0.0000046758632,0.000011109809,0.0003902743,0.00011393186,0.00021014734,0.0016964461,0.000020289594,0.00063789997,0.0000033343351],"about_ca_topic_score_codex":0.002319591,"about_ca_topic_score_gemma":0.004922338,"teacher_disagreement_score":0.002319591,"about_ca_system_score_codex":0.00019114003,"about_ca_system_score_gemma":0.000101800055,"threshold_uncertainty_score":0.004612148},"labels":[],"label_agreement":null},{"id":"W4323669801","doi":"10.3847/1538-4357/acbc7d","title":"A Measurement of Circumgalactic Gas around Nearby Galaxies Using Fast Radio Bursts","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Science Foundation","keywords":"Physics; Halo; Astrophysics; Galaxy; Virial theorem; Stack (abstract data type); Astronomy; Intergalactic medium; Bin; Redshift; Algorithm","score_opus":0.022657181481379123,"score_gpt":0.2352066873316962,"score_spread":0.21254950585031707,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323669801","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99332595,0.00019914344,0.002062947,0.00004926143,0.000007209874,0.000012378626,0.0019084518,0.00018573366,0.002248918],"genre_scores_gemma":[0.9963877,0.000048181413,0.0022389118,0.000020773323,0.000011173658,0.000005463438,0.0011102089,0.000016632388,0.00016099807],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974686,0.000042928994,0.000009754905,0.00008226688,0.000068237096,0.000049925184],"domain_scores_gemma":[0.9986393,0.00029628174,0.0003759294,0.00021876278,0.00014318575,0.00032655735],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047850612,0.00037150865,0.00017408012,0.001503368,0.00019914212,0.0006551335,0.00031560686,0.00026111887,0.0011840656],"category_scores_gemma":[0.001399275,0.0002102406,0.00024878193,0.0008401705,0.00018798841,0.00035185734,0.0005027633,0.00022959075,0.00029558036],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014166463,0.00003797299,0.9613139,0.000033858596,0.00016238462,0.0001008873,0.00024636328,0.0026421335,0.020965507,0.00048433477,0.00062103407,0.013249908],"study_design_scores_gemma":[0.0000068256722,0.000052128104,0.99267757,0.000012622138,0.00003339595,0.000060144936,0.00012953054,0.0033711141,0.0024552685,0.00017135625,0.0010174956,0.0000125922725],"about_ca_topic_score_codex":0.005207379,"about_ca_topic_score_gemma":0.007512725,"teacher_disagreement_score":0.005207379,"about_ca_system_score_codex":0.0003292911,"about_ca_system_score_gemma":0.00011967489,"threshold_uncertainty_score":0.010354161},"labels":[],"label_agreement":null},{"id":"W4323670085","doi":"10.3847/1538-4357/acb925","title":"HectoMAP: The Complete Redshift Survey (Data Release 2)","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Japan Society for the Promotion of Science; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Lawrence Berkeley National Laboratory; Ministry of Science and ICT, South Korea; Universidad Nacional Autónoma de México; National Research Foundation of Korea; Cabinet Office, Government of Japan; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; Natural Sciences and Engineering Research Council of Canada; York University; Leibniz-Gemeinschaft; University of Notre Dame; Toray Science Foundation; High Energy Accelerator Research Organization; Ohio State University; National Research Foundation; Carnegie Mellon University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; Japan Science and Technology Agency; U.S. Department of Energy; Smithsonian Institution; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Vanderbilt University; Seoul National University; Yale University; Ministry of Education, Culture, Sports, Science and Technology; Academia Sinica","keywords":"Physics; Redshift; Astrophysics; Photometry (optics); Galaxy; Redshift survey; Photometric redshift; Sky; Astronomy; Stars","score_opus":0.03650026277120553,"score_gpt":0.2554908288896894,"score_spread":0.21899056611848386,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4323670085","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.017153433,0.00011541298,0.0017399132,0.00010728074,0.000018777922,0.00016043658,0.9723589,0.002233422,0.006112568],"genre_scores_gemma":[0.0248282,0.000065016626,0.002622106,0.00007864027,0.00003258574,0.0002916387,0.969257,0.00042996937,0.0023948865],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9987206,0.00015444898,0.00008622375,0.00025077054,0.00053122157,0.00025676316],"domain_scores_gemma":[0.99574643,0.00029344138,0.00095509127,0.0009848688,0.0012782691,0.0007418932],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001679925,0.0009641879,0.0010771604,0.0065701106,0.00069129677,0.0018837855,0.0019226831,0.0005434495,0.0214966],"category_scores_gemma":[0.0035157255,0.00078429934,0.00043540742,0.011322761,0.00027644346,0.0010941019,0.0025300449,0.0008810456,0.017999234],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085274456,0.00013963977,0.07867078,0.000493079,0.00022065741,0.00021335416,0.000313133,0.0009350965,0.0021671408,0.001774158,0.8675396,0.046680607],"study_design_scores_gemma":[0.00046847234,0.00008023373,0.55700773,0.00008635055,0.00007037249,0.00022839816,0.00021904141,0.0012594792,0.0018243026,0.00081459427,0.43787342,0.000067596055],"about_ca_topic_score_codex":0.05035814,"about_ca_topic_score_gemma":0.034822,"teacher_disagreement_score":0.05035814,"about_ca_system_score_codex":0.000992981,"about_ca_system_score_gemma":0.0018952695,"threshold_uncertainty_score":0.10013008},"labels":[],"label_agreement":null},{"id":"W4324046711","doi":"10.3847/1538-4357/acb055","title":"Examining the Rotation Period Distribution of the 40 Myr Tucana–Horologium Association with TESS","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"National Aeronautics and Space Administration","keywords":"Physics; Rotation (mathematics); Light curve; Rotation period; Astrophysics; Sky; Context (archaeology); Astronomy; Stars; Geometry; Mathematics; Geology; Paleontology","score_opus":0.012627584233366965,"score_gpt":0.2151522058388839,"score_spread":0.20252462160551693,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324046711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99818915,0.00006769224,0.000114913746,0.00001145135,0.000003272826,0.0000033822537,0.00038422976,0.000014107099,0.0012116748],"genre_scores_gemma":[0.9984267,0.000028899201,0.00013083604,0.000004532813,0.000004362199,0.0000030088395,0.0011307797,0.0000073936917,0.00026351132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997862,0.000014297643,0.00000985807,0.00006728974,0.000047312333,0.000075023614],"domain_scores_gemma":[0.99913955,0.000055139208,0.00031496948,0.00010635631,0.00018739974,0.00019671358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041353365,0.00017869013,0.00020076474,0.0019354646,0.00072727655,0.00082180824,0.00026029014,0.00015394783,0.0019215058],"category_scores_gemma":[0.00096902926,0.00008538948,0.00014856468,0.0017211295,0.00041329206,0.00023556844,0.00077611953,0.00017394705,0.0003889096],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008439321,0.000010286512,0.9873147,0.00000839034,0.000027793114,0.00004701079,0.0002738834,0.00021832767,0.0036165991,0.00013165768,0.00043655932,0.0078303935],"study_design_scores_gemma":[9.639076e-7,0.0000068732475,0.9987494,0.0000022840388,0.0000047464473,0.000020938074,0.0001553288,0.00019706874,0.00018568276,0.00001802991,0.00065714517,0.0000015579448],"about_ca_topic_score_codex":0.034146592,"about_ca_topic_score_gemma":0.04926092,"teacher_disagreement_score":0.034146592,"about_ca_system_score_codex":0.0005544852,"about_ca_system_score_gemma":0.00037058562,"threshold_uncertainty_score":0.06789571},"labels":[],"label_agreement":null},{"id":"W4324046843","doi":"10.3847/1538-4357/acb8a9","title":"Circumstellar Medium Interaction in SN 2018lab, A Low-luminosity Type IIP Supernova Observed with TESS","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Heising-Simons Foundation; Nuclear Safety and Security Commission; University of Washington; Agencia Estatal de Investigación; National Aeronautics and Space Administration; California Institute of Technology; Washington Research Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Ejecta; Light curve; Supernova; Luminosity; Red supergiant; Supergiant; Spectral line; Astronomy; Stars; Galaxy","score_opus":0.02572370820788724,"score_gpt":0.24615268218949285,"score_spread":0.2204289739816056,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324046843","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99918073,0.000050759492,0.00008634109,0.000006776689,0.00000289971,0.000002714503,0.00031154716,0.000018531397,0.00033985762],"genre_scores_gemma":[0.99899656,0.000025923524,0.00010525314,0.000008032824,0.000007031428,0.0000027480482,0.0007184064,0.000006656295,0.00012943344],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994135,0.000005034706,0.000006264347,0.00001870028,0.000014293399,0.000014274341],"domain_scores_gemma":[0.9996902,0.00002682983,0.000121278754,0.000030436615,0.00004221931,0.00008911724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015976318,0.00027229372,0.00021073391,0.0010769685,0.00027414085,0.00037962082,0.00017936183,0.00019843927,0.00093306263],"category_scores_gemma":[0.00032905073,0.000101525904,0.00022750364,0.0004890915,0.00018925435,0.00019892026,0.0004729574,0.00017607803,0.00022122372],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039406307,0.00009128009,0.9688301,0.000020283333,0.00004232387,0.0017176615,0.00013038375,0.00015533414,0.021980656,0.00008176061,0.00039452052,0.0061616064],"study_design_scores_gemma":[0.000006936504,0.00012176806,0.99499726,0.000004183532,0.000014356879,0.0021806925,0.00008802164,0.000393559,0.0014646621,0.000055170545,0.00066856167,0.0000049217865],"about_ca_topic_score_codex":0.0022385332,"about_ca_topic_score_gemma":0.0037462676,"teacher_disagreement_score":0.0022385332,"about_ca_system_score_codex":0.00019711115,"about_ca_system_score_gemma":0.000090239766,"threshold_uncertainty_score":0.004450977},"labels":[],"label_agreement":null},{"id":"W4324046858","doi":"10.3847/1538-4357/acbc7b","title":"Search for Ultraheavy Dark Matter from Observations of Dwarf Spheroidal Galaxies with VERITAS","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Office of Science; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Research Foundation; National Energy Research Scientific Computing Center; National Research Foundation of Korea; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Physics; Dark matter; Astrophysics; Weakly interacting massive particles; WIMP; Astronomy; Galaxy; Dwarf galaxy; Light dark matter; Warm dark matter; Dwarf spheroidal galaxy; Scalar field dark matter; Dwarf galaxy problem; Mixed dark matter; Annihilation; Particle physics; Dark matter halo; Dark energy; Cosmology; Interacting galaxy; Halo","score_opus":0.020578366177230537,"score_gpt":0.24285859311272717,"score_spread":0.22228022693549665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324046858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998648,0.00003418957,0.0004778103,0.000018103407,0.0000016756642,0.0000033388885,0.00039720946,0.00003220302,0.00038744218],"genre_scores_gemma":[0.9983689,0.00001036283,0.0005815688,0.000008262087,0.0000030091335,0.0000022188317,0.00088910304,0.000006016996,0.00013052151],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995634,0.00006786034,0.00002099679,0.00014835838,0.000101861995,0.00009752841],"domain_scores_gemma":[0.99806815,0.00047558974,0.0006642447,0.00036309304,0.000108569584,0.00032024973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008150813,0.00026278695,0.0003087799,0.0012169454,0.00035193784,0.0007438414,0.0005176656,0.00024841784,0.002071568],"category_scores_gemma":[0.0011308634,0.00024035462,0.0003925964,0.00074990076,0.00029609769,0.00023874556,0.0009827637,0.0003095758,0.00022424206],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002710619,0.000033178705,0.9641702,0.00001993875,0.0001498643,0.00026639822,0.00016802133,0.0012071904,0.027626682,0.0004378806,0.0002609849,0.0053884718],"study_design_scores_gemma":[0.0000123209375,0.00005801255,0.9936386,0.000007042669,0.00003776245,0.00015640403,0.000101332116,0.0032762564,0.002040075,0.00011762862,0.00054865424,0.0000059530125],"about_ca_topic_score_codex":0.009765225,"about_ca_topic_score_gemma":0.0239415,"teacher_disagreement_score":0.009765225,"about_ca_system_score_codex":0.00046781675,"about_ca_system_score_gemma":0.0004092652,"threshold_uncertainty_score":0.01941681},"labels":[],"label_agreement":null},{"id":"W4324096662","doi":"10.3847/1538-4357/acbc7c","title":"The 2022 High-energy Outburst and Radio Disappearing Act of the Magnetar 1E 1547.0–5408","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Precursory Research for Embryonic Science and Technology; Goddard Space Flight Center; Swinburne University of Technology; Centre National d’Etudes Spatiales; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Oak Ridge Associated Universities; University of Maryland, Baltimore County; National Aeronautics and Space Administration; National Science Foundation","keywords":"Magnetar; Astrophysics; Physics; Radio telescope; Glitch; Neutron star; Astronomy","score_opus":0.008307093291390951,"score_gpt":0.2679457270093025,"score_spread":0.25963863371791157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324096662","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977925,0.00023210209,0.00016361536,0.00011785436,0.000037284204,0.000007459465,0.00012209616,0.000025560721,0.0015015487],"genre_scores_gemma":[0.998393,0.000061430816,0.00023697416,0.00011479075,0.00005457734,0.00000734418,0.0004394376,0.000014615483,0.0006778383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998889,0.000009570088,0.0000062074637,0.000028736767,0.00003272628,0.0000338494],"domain_scores_gemma":[0.99958926,0.00003216045,0.000119405246,0.000045578017,0.0000620997,0.00015150366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027323177,0.00027466932,0.00041486567,0.00047559472,0.0006160529,0.0004936702,0.0003191905,0.0004760739,0.00095471303],"category_scores_gemma":[0.00045871982,0.00017272499,0.00024404752,0.00016601472,0.00037198942,0.00023288235,0.00086267147,0.000674071,0.0004892666],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010795196,0.00026191043,0.6532927,0.00012048259,0.00014244136,0.010025869,0.0010483944,0.00032255976,0.30841362,0.0005646596,0.0026058997,0.022121955],"study_design_scores_gemma":[0.000017158301,0.00027042176,0.99099404,0.000011853298,0.000024894045,0.0018238659,0.00021652789,0.00022929042,0.002573387,0.000093489834,0.0037324552,0.000012580415],"about_ca_topic_score_codex":0.0013304144,"about_ca_topic_score_gemma":0.003085409,"teacher_disagreement_score":0.0013304144,"about_ca_system_score_codex":0.00036226978,"about_ca_system_score_gemma":0.00010816316,"threshold_uncertainty_score":0.0031938553},"labels":[],"label_agreement":null},{"id":"W4324139215","doi":"10.3847/1538-4357/acb8b7","title":"The Oceanus Moving Group: A New 500 Myr Old Host for the Nearest Brown Dwarf","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; myr; Brown dwarf; Astrophysics; Astronomy; Astrobiology; Stars; Genetics","score_opus":0.016718461547081682,"score_gpt":0.23650066869711106,"score_spread":0.21978220715002939,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324139215","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975617,0.00014395673,0.00054356223,0.00004578997,0.000028857181,0.0000075265893,0.00011955997,0.000039492774,0.0015095243],"genre_scores_gemma":[0.9977774,0.000037168047,0.00089643965,0.000041092186,0.000028699556,0.0000031687737,0.000281609,0.000012878002,0.0009215298],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998753,0.000006463992,0.0000050231224,0.00004352703,0.000028591932,0.000041082563],"domain_scores_gemma":[0.9997135,0.000020197718,0.000067705165,0.00004394485,0.00002776069,0.00012693072],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016986673,0.00015630217,0.00024571572,0.00071878085,0.0008214955,0.00047645663,0.00024747767,0.00020652327,0.0017826563],"category_scores_gemma":[0.00031407483,0.00009746014,0.00013727896,0.0003148213,0.00038488163,0.00026916948,0.0008085626,0.00027160198,0.0006343872],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033895014,0.000077323304,0.8919981,0.000050535964,0.00004431978,0.0023409005,0.001507423,0.00014409077,0.070402,0.0017074435,0.0012370396,0.030151911],"study_design_scores_gemma":[0.000015741238,0.00024235422,0.9706664,0.000018299605,0.000033270502,0.0038301437,0.00086275476,0.00069781207,0.003733406,0.00061579933,0.019266894,0.000017013826],"about_ca_topic_score_codex":0.0020113306,"about_ca_topic_score_gemma":0.0026562475,"teacher_disagreement_score":0.0020113306,"about_ca_system_score_codex":0.0002172911,"about_ca_system_score_gemma":0.00015015106,"threshold_uncertainty_score":0.005963564},"labels":[],"label_agreement":null},{"id":"W4324139219","doi":"10.3847/1538-4357/acaf50","title":"Improved Constraints on the 21 cm EoR Power Spectrum and the X-Ray Heating of the IGM with HERA Phase I Observations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":175,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Gordon and Betty Moore Foundation; Science and Technology Facilities Council; National Science Foundation","keywords":"Reionization; Physics; HERA; Astrophysics; Metallicity; Stars; Luminosity; Redshift; Galaxy; Particle physics; Quantum chromodynamics","score_opus":0.013212826402531873,"score_gpt":0.22969251492667236,"score_spread":0.21647968852414048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324139219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95585847,0.0005464768,0.03470074,0.0003608493,0.000021468602,0.000019387831,0.0026488153,0.00051236677,0.005331543],"genre_scores_gemma":[0.9904895,0.00008690301,0.007162307,0.000070594804,0.000028859677,0.000014188732,0.00174218,0.000060265458,0.00034533345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99885154,0.00048159974,0.000040595718,0.0002597072,0.00022599415,0.00014059033],"domain_scores_gemma":[0.9934268,0.0034434933,0.0013195041,0.0012118825,0.00037951994,0.00021876625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004113043,0.0006617971,0.00042597635,0.0009620476,0.00027211415,0.0011290234,0.00063731906,0.0003418307,0.0021556078],"category_scores_gemma":[0.0069741346,0.0003365661,0.00074098207,0.00071483006,0.00028608306,0.00089093525,0.0011548062,0.00056520134,0.00043104048],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00069926336,0.0001096744,0.79441714,0.00014825564,0.0004886913,0.00035805456,0.0002530705,0.11947126,0.03220295,0.0054746643,0.0024108954,0.04396602],"study_design_scores_gemma":[0.0000734564,0.00013384722,0.7831679,0.000075623546,0.00023714008,0.0002072189,0.0001862829,0.1774364,0.023973186,0.007299024,0.0071229334,0.000086952234],"about_ca_topic_score_codex":0.0035572385,"about_ca_topic_score_gemma":0.0033436872,"teacher_disagreement_score":0.004113043,"about_ca_system_score_codex":0.0003935992,"about_ca_system_score_gemma":0.0002743681,"threshold_uncertainty_score":0.021752119},"labels":[],"label_agreement":null},{"id":"W4324139289","doi":"10.3847/1538-4357/acb931","title":"VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"Science and Technology Facilities Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Physics; Jansky; Astrophysics; Submillimeter Array; Redshift; Galaxy; Millimeter; Star formation; Astronomy; Mass ratio; Stellar mass; Radio galaxy","score_opus":0.010891822883524426,"score_gpt":0.22548371194908573,"score_spread":0.21459188906556131,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324139289","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981914,0.00013960268,0.00011470313,0.000026703876,0.0000016030425,0.0000042447346,0.00092821725,0.000020063646,0.000573394],"genre_scores_gemma":[0.99789065,0.00009754058,0.0001975403,0.000024888304,0.000009836378,0.000005074471,0.0014992452,0.0000046188607,0.0002705154],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998017,0.00002915905,0.000010497408,0.0000590964,0.00004958381,0.000049958406],"domain_scores_gemma":[0.99882406,0.000111714035,0.00038325874,0.00011168484,0.00015108264,0.0004181399],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005653304,0.0001770224,0.00026759223,0.001836573,0.00037176925,0.00059401465,0.00035141985,0.00018825423,0.0009942752],"category_scores_gemma":[0.00080023875,0.00012312613,0.00016243999,0.0010946535,0.00022730956,0.00033054673,0.0006358421,0.00023921656,0.0004287276],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000025270629,0.000023671939,0.99529535,0.0000055031164,0.00002156072,0.00002721027,0.00009517881,0.00004601814,0.0023729894,0.000039429025,0.000121137746,0.0019266582],"study_design_scores_gemma":[9.420091e-7,0.000012780381,0.9996195,0.0000010757403,0.0000041444528,0.000025023583,0.000036769277,0.000049994575,0.00009963243,0.0000062368454,0.0001430821,7.282712e-7],"about_ca_topic_score_codex":0.009445945,"about_ca_topic_score_gemma":0.013342606,"teacher_disagreement_score":0.009445945,"about_ca_system_score_codex":0.00031203934,"about_ca_system_score_gemma":0.00018574092,"threshold_uncertainty_score":0.0187819},"labels":[],"label_agreement":null},{"id":"W4324139336","doi":"10.3847/1538-4357/acb772","title":"A Catalog of 71 Coronal Line Galaxies in MaNGA: [Ne v] Is an Effective AGN Tracer","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Colorado State University; University of Leicester; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Astronomy; Lambda; Sky; Star formation; Luminous infrared galaxy; Observatory; Line (geometry); Emission spectrum; Spectral line","score_opus":0.010262204277414136,"score_gpt":0.23889591004185148,"score_spread":0.22863370576443734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324139336","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9935314,0.00040869525,0.0004848884,0.000053717034,0.000005633065,0.000017872178,0.0036532183,0.00014091464,0.0017036069],"genre_scores_gemma":[0.9937541,0.00016679951,0.0010512697,0.000032531196,0.000013215561,0.000014479946,0.0045369877,0.00002405662,0.00040657676],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996387,0.000034564477,0.000024701858,0.00013136328,0.000095010306,0.00007575676],"domain_scores_gemma":[0.9976295,0.0003429222,0.0008933132,0.00034303276,0.00034582044,0.00044543593],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051644334,0.00022646741,0.00028581318,0.003115472,0.00054995104,0.0009301915,0.00040986371,0.0001811607,0.0013967755],"category_scores_gemma":[0.0016314681,0.00016784997,0.00018843164,0.002309637,0.00031510237,0.00040779368,0.0005863581,0.0001823002,0.0007342835],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002307592,0.000016703432,0.9893321,0.000023017259,0.000020278476,0.000048769656,0.00012341201,0.000121888974,0.0019840992,0.00008488748,0.00078097853,0.0074408194],"study_design_scores_gemma":[0.0000016918165,0.000011161517,0.99770004,0.0000104768205,0.000009424199,0.00008179694,0.00009685599,0.00038038098,0.00031280142,0.000039022932,0.0013527385,0.0000036370266],"about_ca_topic_score_codex":0.010501719,"about_ca_topic_score_gemma":0.017703904,"teacher_disagreement_score":0.010501719,"about_ca_system_score_codex":0.00042803763,"about_ca_system_score_gemma":0.00030473733,"threshold_uncertainty_score":0.020881176},"labels":[],"label_agreement":null},{"id":"W4324139350","doi":"10.3847/1538-4357/acb68b","title":"First Observations of the Brown Dwarf HD 19467 B with JWST","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science Mission Directorate; Goddard Space Flight Center; National Aeronautics and Space Administration; California Institute of Technology; Jet Propulsion Laboratory; Alfred P. Sloan Foundation; Research Corporation for Science Advancement; National Science Foundation","keywords":"Physics; Brown dwarf; Circumbinary planet; Astrophysics; Astronomy; Stars","score_opus":0.02205010612662974,"score_gpt":0.21897412254713997,"score_spread":0.19692401642051022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324139350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969843,0.00014779264,0.00041749675,0.000027870366,0.000014417538,0.000008719064,0.00024893045,0.000040544877,0.002109903],"genre_scores_gemma":[0.9970028,0.00004464079,0.001505383,0.00004624428,0.000019444844,0.0000046300565,0.00074872165,0.000014777881,0.00061332935],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988294,0.0000073238666,0.000007420325,0.000023914572,0.000053659438,0.000024744773],"domain_scores_gemma":[0.99975675,0.00002614306,0.000027006341,0.000038166705,0.00006607483,0.000085858635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019227643,0.00010745444,0.00017978836,0.0006693553,0.00061838713,0.0003086463,0.00020875965,0.00020066428,0.0012045767],"category_scores_gemma":[0.00033806,0.00017722102,0.00013870449,0.00041155666,0.000312376,0.00024956494,0.00071429036,0.00031231673,0.00031423295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007807166,0.00033636903,0.6347442,0.00014494229,0.00019943713,0.0025455442,0.0014478728,0.0006376634,0.2901098,0.0012948279,0.003959421,0.063799195],"study_design_scores_gemma":[0.000022874088,0.00020207277,0.9823235,0.000013801979,0.000029710549,0.0005297266,0.00020936555,0.00058896135,0.008223971,0.00013579844,0.0077113262,0.000008903895],"about_ca_topic_score_codex":0.004287367,"about_ca_topic_score_gemma":0.012681477,"teacher_disagreement_score":0.004287367,"about_ca_system_score_codex":0.00030019734,"about_ca_system_score_gemma":0.00018466022,"threshold_uncertainty_score":0.008524835},"labels":[],"label_agreement":null},{"id":"W4324139359","doi":"10.3847/1538-4357/acba95","title":"Resolving the Emission Regions of the Crab Pulsar’s Giant Pulses. II. Evidence for Relativistic Motion","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Joint Research Fund for Overseas Chinese Scholars and Scholars in Hong Kong and Macao; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Killam Trusts; Ministry of Science and Technology, Taiwan; University of Toronto; Government of Ontario; National Natural Science Foundation of China; Ontario Research Foundation; Canadian Institute for Advanced Research; Alexander von Humboldt-Stiftung; National Science Foundation","keywords":"Physics; Pulsar; Crab Pulsar; Astrophysics; Astronomy; Proper motion; Stars","score_opus":0.054403449722599924,"score_gpt":0.366083975084375,"score_spread":0.3116805253617751,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324139359","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974475,0.0003622369,0.0010561938,0.000039611175,0.0000022995707,0.0000025984093,0.00010849866,0.000020535255,0.0009606085],"genre_scores_gemma":[0.9989802,0.00006640226,0.0006904341,0.000015126593,0.000007350035,0.0000020080718,0.00013047608,0.000008908033,0.0000990603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992,0.0000073186784,0.000004773299,0.000026152267,0.000020220396,0.000021537395],"domain_scores_gemma":[0.99907804,0.00027956598,0.00034695433,0.000095228905,0.00012407583,0.00007614687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031322174,0.00019458905,0.00016457385,0.0010326161,0.00034415838,0.0005512877,0.00032348707,0.00029588433,0.0007747152],"category_scores_gemma":[0.0010880184,0.00019517288,0.00013605696,0.0006947344,0.0002772884,0.00040418777,0.00046835575,0.00026303635,0.00021529236],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029382703,0.000059481703,0.7748858,0.000084991145,0.00008801631,0.00069078634,0.0006260388,0.0013851725,0.19384257,0.000898449,0.00047794735,0.026666995],"study_design_scores_gemma":[0.0000065878444,0.000045445377,0.98761964,0.0000075263747,0.000019859219,0.0006419378,0.0002033875,0.002359416,0.007974985,0.00029177734,0.0008198299,0.000009626555],"about_ca_topic_score_codex":0.001168882,"about_ca_topic_score_gemma":0.0016935864,"teacher_disagreement_score":0.001168882,"about_ca_system_score_codex":0.00020732747,"about_ca_system_score_gemma":0.00012520934,"threshold_uncertainty_score":0.0025916696},"labels":[],"label_agreement":null},{"id":"W4324139431","doi":"10.3847/1538-4357/acba0e","title":"A Broadband X-Ray Study of the Rabbit Pulsar Wind Nebula Powered by PSR J1418-6058","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Pulsar wind nebula; Pulsar; Astrophysics; Spectral index; Astronomy; Nebula; Photon; Spectral line; Optics; Stars","score_opus":0.008101574920192317,"score_gpt":0.22735456369737475,"score_spread":0.21925298877718244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4324139431","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99946314,0.00007523965,0.00012902226,0.0000030760973,0.0000010176225,0.0000022262686,0.000032092794,0.000003593305,0.0002905893],"genre_scores_gemma":[0.99947935,0.000063082734,0.00017946653,0.0000051236343,0.000003330028,0.000002625656,0.00010561377,0.0000031506668,0.00015819886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994123,0.0000064274486,0.0000050233293,0.000021918122,0.000013633797,0.000011820286],"domain_scores_gemma":[0.9998549,0.000022199665,0.0000518605,0.000021143793,0.000018331388,0.000031471067],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018210319,0.00024231462,0.0003698314,0.00053082086,0.00022466194,0.00033896766,0.00022770587,0.00017277045,0.00060842984],"category_scores_gemma":[0.00027817176,0.00019193336,0.00026793077,0.0003042496,0.00019829685,0.00023740405,0.00030864833,0.00014551873,0.00020195778],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045749402,0.00012721086,0.679861,0.0000814325,0.00014780987,0.0024822962,0.00026182228,0.0011904656,0.30441684,0.0004116934,0.000116992705,0.01044481],"study_design_scores_gemma":[0.000021293512,0.00046963152,0.9823934,0.0000110464125,0.00006571874,0.002213193,0.00012680033,0.004159782,0.009185858,0.0001603683,0.0011848697,0.000007955765],"about_ca_topic_score_codex":0.0010082033,"about_ca_topic_score_gemma":0.0010758389,"teacher_disagreement_score":0.0010082033,"about_ca_system_score_codex":0.00012389601,"about_ca_system_score_gemma":0.00006156541,"threshold_uncertainty_score":0.002035439},"labels":[],"label_agreement":null},{"id":"W4327626958","doi":"10.3847/1538-4357/acbc74","title":"Color Gradients and Half-mass Radii of Galaxies Out to z = 2 in the CANDELS/3D-HST Fields: Further Evidence for Important Differences in the Evolution of Mass-weighted and Light-weighted Sizes","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":41,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Galaxy; Redshift; Astrophysics; Stellar mass; Analytical Chemistry (journal); Star formation; Chemistry","score_opus":0.01813522344660143,"score_gpt":0.24616142324681806,"score_spread":0.22802619980021663,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4327626958","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972631,0.00004337127,0.00019755165,0.000044312183,0.0000014088372,0.0000022300303,0.0013035514,0.000043425567,0.0011010254],"genre_scores_gemma":[0.99780375,0.000015064092,0.00017021272,0.00001692797,0.0000043906784,0.0000023177888,0.0016296728,0.000021103275,0.00033652998],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975544,0.000035738663,0.000011993189,0.00007447071,0.000046636684,0.000075768796],"domain_scores_gemma":[0.9958923,0.000995134,0.001023466,0.0004861714,0.00060646195,0.000996438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006467254,0.00017393345,0.00020962888,0.0025095267,0.0002737731,0.00077963836,0.00042652592,0.00024002578,0.0032273524],"category_scores_gemma":[0.0027299826,0.00020391363,0.0002627421,0.0011047496,0.0004977538,0.00062504516,0.00064900256,0.00029181511,0.0009178695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010947322,0.000020068559,0.99278075,0.0000050847643,0.000018783106,0.00002244265,0.00020206961,0.00027030052,0.0026369162,0.00020926124,0.00030402906,0.0034208605],"study_design_scores_gemma":[0.0000011009697,0.0000027104586,0.9994234,7.947416e-7,0.0000016866818,0.000007372191,0.00004364121,0.00026326824,0.000139593,0.000030604915,0.00008433607,0.0000015354044],"about_ca_topic_score_codex":0.023548223,"about_ca_topic_score_gemma":0.023721546,"teacher_disagreement_score":0.023548223,"about_ca_system_score_codex":0.00039063086,"about_ca_system_score_gemma":0.00019393484,"threshold_uncertainty_score":0.04682231},"labels":[],"label_agreement":null},{"id":"W4327626985","doi":"10.3847/1538-4357/acbc26","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Density Structure of Centrally Concentrated Prestellar Cores from Multiscale Observations ","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Science and Technology Council; Academia Sinica; National Radio Astronomy Observatory; National Natural Science Foundation of China; Chinese Academy of Sciences; Science and Engineering Research Board; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Millimeter; Stars; Star formation; Submillimeter Array; Astronomy","score_opus":0.025912428341439864,"score_gpt":0.24585718198542078,"score_spread":0.21994475364398092,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4327626985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992855,0.000036648376,0.00016592412,0.0000075953026,7.9542195e-7,0.000003534735,0.00025958798,0.000015952133,0.00022442531],"genre_scores_gemma":[0.99902844,0.000019063315,0.000379126,0.0000061946143,0.000003083869,0.0000036863487,0.0004892203,0.000004225678,0.00006690547],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999213,0.000008798572,0.000004022878,0.00003128764,0.000018957287,0.000015638638],"domain_scores_gemma":[0.99975973,0.000026902593,0.0000785597,0.000043650693,0.000035194706,0.000056059293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022759584,0.0001700197,0.00013854561,0.00073319755,0.00023213815,0.00029007703,0.00031976769,0.00015940529,0.0003884827],"category_scores_gemma":[0.0003626025,0.00012327978,0.00018845015,0.00042413635,0.00013380362,0.00020205813,0.0004236725,0.00012071455,0.00012165413],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059973285,0.000040432118,0.9787184,0.000017719261,0.00006172539,0.00013389948,0.00019809153,0.0016089805,0.012508271,0.00012864971,0.0003039958,0.0062198066],"study_design_scores_gemma":[0.0000042692072,0.000012662326,0.9944622,0.000002295169,0.000008130425,0.00003289878,0.000057751608,0.0045350147,0.00056216767,0.000026678246,0.000293033,0.0000027883912],"about_ca_topic_score_codex":0.010889105,"about_ca_topic_score_gemma":0.01689324,"teacher_disagreement_score":0.010889105,"about_ca_system_score_codex":0.00026402908,"about_ca_system_score_gemma":0.00016166538,"threshold_uncertainty_score":0.021651447},"labels":[],"label_agreement":null},{"id":"W4327985486","doi":"10.3847/1538-4357/acbd45","title":"The Messy Nature of Fiber Spectra: Star–Quasar Pairs Masquerading as Dual Type 1 AGNs","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; York University; Istituto Nazionale di Astrofisica; Arizona Board of Regents; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Office of Science; College of Engineering, Michigan State University; Princeton University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Goddard Space Flight Center; Harvard University; New Mexico State University; University of Portsmouth; Oak Ridge Associated Universities; Yale University; Vanderbilt University; Ohio State University; University of Minnesota; National Science Foundation; Leibniz-Institut für Astrophysik Potsdam; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Physics; Astrophysics; Active galactic nucleus; Supermassive black hole; Stars; Spectral line; Quasar; Emission spectrum; Astronomy; Galaxy","score_opus":0.007620690361577892,"score_gpt":0.2285541288543793,"score_spread":0.22093343849280142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4327985486","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99895966,0.000034535202,0.00029110955,0.000010851355,0.0000018614137,0.0000040283794,0.00008205353,0.00001580297,0.00060000195],"genre_scores_gemma":[0.99956137,0.000011048481,0.0002236978,0.000007674517,0.000004310963,0.0000017003026,0.00009501511,0.0000024989658,0.00009271145],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977106,0.000025663754,0.000019100788,0.00007658692,0.000052684325,0.000054891174],"domain_scores_gemma":[0.99906033,0.00013922992,0.0004617526,0.000081642844,0.00009370741,0.00016336427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003702459,0.00021885053,0.00017200052,0.0018112184,0.00046211545,0.0006002714,0.00021734498,0.0001721131,0.0022721046],"category_scores_gemma":[0.0007781046,0.000109331835,0.00011759245,0.0006279111,0.00033168218,0.00043007202,0.00063229114,0.00015103228,0.00031095897],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014678136,0.000026369304,0.95958924,0.0000121032035,0.000037250782,0.0010483309,0.00033127234,0.00006556766,0.03295317,0.00015146323,0.00012681817,0.0055116788],"study_design_scores_gemma":[0.0000027058684,0.000044917237,0.99398226,0.0000022100983,0.000016508708,0.0024184512,0.00037029697,0.00030881984,0.0024386146,0.00012197399,0.00028920447,0.0000038967964],"about_ca_topic_score_codex":0.00088953064,"about_ca_topic_score_gemma":0.0016148353,"teacher_disagreement_score":0.0022721046,"about_ca_system_score_codex":0.00015519709,"about_ca_system_score_gemma":0.00006878707,"threshold_uncertainty_score":0.0076009035},"labels":[],"label_agreement":null},{"id":"W4328089518","doi":"10.3847/1538-4357/acbafc","title":"A Candidate Relativistic Tidal Disruption Event at 340 Mpc","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Saha Institute of Nuclear Physics, Department of Atomic Energy, Government of India; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Accretion (finance); Flare; Supermassive black hole; Astronomy; Sky; Active galactic nucleus; Redshift; Jet (fluid); Astrophysical jet; Galaxy; RADIUS; Luminosity","score_opus":0.013991787503110892,"score_gpt":0.25678498410341044,"score_spread":0.24279319660029955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4328089518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9928907,0.00016457734,0.0010772232,0.0002178666,0.00004666036,0.000016920598,0.0006521102,0.00016175224,0.0047721076],"genre_scores_gemma":[0.99840826,0.000018379575,0.00035883047,0.00004764422,0.000023133513,0.0000031348052,0.00055749196,0.000007123473,0.00057610346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999263,0.000003880064,0.0000027485971,0.000022490583,0.000014170611,0.000030316818],"domain_scores_gemma":[0.9998497,0.0000075221064,0.000047825757,0.000014965459,0.000016202104,0.000063809486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000999531,0.00016892281,0.0001722129,0.0005122803,0.00066068256,0.00049804786,0.00032382988,0.00044633367,0.002891204],"category_scores_gemma":[0.00023540678,0.00013316721,0.00020127016,0.0003535744,0.00016037232,0.00019281878,0.0005160519,0.0003641682,0.0005039652],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047460594,0.00028019477,0.8927076,0.00004420044,0.00011441304,0.01225308,0.00051402196,0.0023817874,0.056793693,0.0036880998,0.006865889,0.023882505],"study_design_scores_gemma":[0.000021161906,0.0001064959,0.98459756,0.000010094765,0.000020868261,0.0016848049,0.00015929036,0.0043769544,0.0017143212,0.0006349622,0.006657667,0.000015757389],"about_ca_topic_score_codex":0.005575524,"about_ca_topic_score_gemma":0.0073787468,"teacher_disagreement_score":0.005575524,"about_ca_system_score_codex":0.00037335439,"about_ca_system_score_gemma":0.00014488904,"threshold_uncertainty_score":0.011086166},"labels":[],"label_agreement":null},{"id":"W4328093772","doi":"10.3847/1538-4357/acb8b2","title":"The Missing Link between Black Holes in High-mass X-Ray Binaries and Gravitational-wave Sources: Observational Selection Effects","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; Canadian Institute for Advanced Research; Northwestern University; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Binary black hole; Gravitational wave; Redshift; Astronomy; High mass; Merge (version control); Population; Galaxy","score_opus":0.02612965275456742,"score_gpt":0.24940679995973003,"score_spread":0.22327714720516262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4328093772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955918,0.0003519608,0.0019673023,0.00034453665,0.000012647536,0.0000067942447,0.00012385198,0.000022915623,0.0015780394],"genre_scores_gemma":[0.999734,0.000029452334,0.000117872485,0.000024751282,0.000012311116,7.191375e-7,0.00003145136,0.0000022585127,0.000047172947],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993498,0.00027382086,0.00004807358,0.00013590828,0.00011919701,0.000073073265],"domain_scores_gemma":[0.9810627,0.0120929945,0.0039920984,0.001163753,0.0005300262,0.0011583872],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003052456,0.00023482686,0.0003450451,0.00059353444,0.00053793995,0.0011772605,0.00068997836,0.0006113735,0.0035981438],"category_scores_gemma":[0.01227528,0.0001746021,0.0003657544,0.0005549333,0.001045359,0.0010296548,0.0007491926,0.00042008838,0.00020889923],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021499982,0.000050123457,0.9868564,0.00003359537,0.00014698393,0.00016182393,0.000058719805,0.0032783512,0.0013674753,0.0019619712,0.00017060814,0.0056989663],"study_design_scores_gemma":[0.000082578794,0.00014085007,0.9391109,0.00003144049,0.00019241736,0.00035377944,0.00022492201,0.051791918,0.0013475664,0.0061695906,0.00053292833,0.000021159462],"about_ca_topic_score_codex":0.0026723528,"about_ca_topic_score_gemma":0.002740835,"teacher_disagreement_score":0.0035981438,"about_ca_system_score_codex":0.00026718486,"about_ca_system_score_gemma":0.00023247063,"threshold_uncertainty_score":0.016143143},"labels":[],"label_agreement":null},{"id":"W4353074885","doi":"10.3847/1538-4357/acafe7","title":"A Systematic View of Ten New Black Hole Spins","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":59,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"National Aeronautics and Space Administration","keywords":"Physics; Spins; Astrophysics; Astronomy; Black hole (networking); Theoretical physics; Condensed matter physics","score_opus":0.019505065787123795,"score_gpt":0.251222337287602,"score_spread":0.23171727150047822,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4353074885","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9950494,0.000248673,0.0010569046,0.00003724221,0.000007700294,0.000009143192,0.0003631319,0.00006532928,0.0031624772],"genre_scores_gemma":[0.9974131,0.00007412949,0.001537946,0.000025377974,0.000011343174,0.000009303346,0.00047597205,0.000014339731,0.0004385299],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995908,0.00006914044,0.00002849197,0.00015335,0.000107258216,0.000051017003],"domain_scores_gemma":[0.9979073,0.0003739863,0.000825744,0.00034078836,0.00038349425,0.00016868993],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006872634,0.00022398541,0.00023417064,0.0022245625,0.00050246937,0.0006994855,0.00036193925,0.00024062635,0.0015882418],"category_scores_gemma":[0.0017450525,0.000245593,0.0001807423,0.0008968718,0.00055410503,0.0005425145,0.0007193338,0.00026291976,0.00032689763],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016095879,0.00003706684,0.943192,0.00008198798,0.00007924268,0.000119403805,0.0010819741,0.0002622372,0.028319992,0.0012586851,0.0005670921,0.024839383],"study_design_scores_gemma":[0.000008255911,0.000091031936,0.9883829,0.00001903246,0.000045867724,0.00023894364,0.0003142323,0.0012206695,0.0067674685,0.0005860217,0.0023095626,0.00001602159],"about_ca_topic_score_codex":0.0013194713,"about_ca_topic_score_gemma":0.0040457924,"teacher_disagreement_score":0.0022245625,"about_ca_system_score_codex":0.0003753151,"about_ca_system_score_gemma":0.00016379938,"threshold_uncertainty_score":0.0053132176},"labels":[],"label_agreement":null},{"id":"W4353097453","doi":"10.3847/1538-4357/acb6f5","title":"Chemodynamical Analysis of Metal-rich High-eccentricity Stars in the Milky Way's Disk","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of International Science and Engineering; National Astronomical Observatories, Chinese Academy of Sciences; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Lawrence Berkeley National Laboratory; Ministry of Science and ICT, South Korea; Ministério da Ciência, Tecnologia e Inovação; Chinese Academy of Sciences; University of Oxford; York University; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Leibniz-Gemeinschaft; University of Notre Dame; National Development and Reform Commission; Ohio State University; National Research Foundation; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Astrophysics; Stars; Milky Way; Thick disk; Astronomy; Population; LAMOST; Galactic halo; Accretion (finance); Halo; Galaxy","score_opus":0.01092829983506198,"score_gpt":0.2330099368300528,"score_spread":0.22208163699499084,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4353097453","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999764,0.000036617494,0.00002258386,0.0000033693118,2.791464e-7,0.0000013526958,0.00007594082,0.000001812935,0.000094070514],"genre_scores_gemma":[0.9995466,0.000027777054,0.000063061765,0.0000040206683,0.000001619828,0.0000016107532,0.00026766956,0.0000013105588,0.00008628116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998652,0.000013523211,0.000014084624,0.00004504639,0.000028205983,0.000033958528],"domain_scores_gemma":[0.99950874,0.000054352182,0.00018913692,0.000041874133,0.00008543602,0.00012052879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016905609,0.00019801062,0.00025859132,0.0028307927,0.00037317484,0.00055961916,0.00024201444,0.00019488114,0.0005392429],"category_scores_gemma":[0.00048595513,0.00013758916,0.00025840866,0.0017052079,0.00030148917,0.0002524256,0.000672119,0.0000831305,0.00018069577],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004683921,0.000011343004,0.992063,0.000008168346,0.000030216526,0.00009302802,0.00011724458,0.000113767346,0.0056270286,0.000022902947,0.000026370886,0.0018401501],"study_design_scores_gemma":[0.0000011309477,0.000012141615,0.9993782,6.7897867e-7,0.000005522667,0.000059367074,0.000088864144,0.00014916927,0.0002285438,0.000007510411,0.00006783405,0.0000010270612],"about_ca_topic_score_codex":0.006044496,"about_ca_topic_score_gemma":0.0078596845,"teacher_disagreement_score":0.006044496,"about_ca_system_score_codex":0.00037790445,"about_ca_system_score_gemma":0.00017551465,"threshold_uncertainty_score":0.012018621},"labels":[],"label_agreement":null},{"id":"W4353106018","doi":"10.3847/1538-4357/aca9be","title":"The Origin and Evolution of the Normal Type Ia SN 2018aoz with Infant-phase Reddening and Excess Emission","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"European Social Fund; Fondo Nacional de Desarrollo Científico y Tecnológico; High Energy Physics; Fundação para a Ciência e a Tecnologia; European Research Council; Natural Sciences and Engineering Research Council of Canada; Office of Science; Ministry of Science and ICT, South Korea; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Ministerio de Ciencia e Innovación; Agencia Nacional de Investigación y Desarrollo; National Research Foundation of Korea; Stavros Niarchos Foundation; National Energy Research Scientific Computing Center; Nuclear Safety and Security Commission; Heising-Simons Foundation; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; University of Toronto; National Research Foundation; W. M. Keck Foundation; Israel Science Foundation; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; Hellenic Foundation for Research and Innovation; U.S. Department of Energy; California Institute of Technology; Canada Research Chairs; National Science Foundation","keywords":"Physics; Astrophysics; Ejecta; White dwarf; Supernova; Luminosity; Phase (matter); Pair-instability supernova; Torus; Light curve; Galaxy; Stars","score_opus":0.009560265392248194,"score_gpt":0.2585255030702749,"score_spread":0.2489652376780267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4353106018","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99694425,0.00008448392,0.00042981651,0.000039764607,0.000008236846,0.00000929914,0.0001784473,0.000028466387,0.0022773664],"genre_scores_gemma":[0.9985916,0.000042223022,0.00027728887,0.000013042737,0.0000074436994,0.0000060971656,0.0003906101,0.000008639479,0.00066297257],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999485,0.0000036398808,0.0000028314405,0.0000150949745,0.000014845168,0.000015012369],"domain_scores_gemma":[0.9998474,0.000011538892,0.0000667996,0.000011746788,0.00002686452,0.00003568194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013031023,0.00023046542,0.00013553578,0.00068163866,0.00029284356,0.0005642465,0.00026245668,0.00028682261,0.0020384213],"category_scores_gemma":[0.0003953271,0.00010603552,0.00020754641,0.0002370417,0.0002607283,0.00020910488,0.00044535275,0.00020416128,0.00063841394],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014842124,0.000042011434,0.96675116,0.000017148575,0.00003059246,0.0010615672,0.00012277252,0.00026975424,0.018301515,0.0013043736,0.00049591984,0.011454763],"study_design_scores_gemma":[0.000007600409,0.000059590424,0.99286,0.000008152043,0.000012695521,0.0014297338,0.0001165405,0.0012967371,0.001200011,0.00064378715,0.0023607875,0.000004380172],"about_ca_topic_score_codex":0.002456794,"about_ca_topic_score_gemma":0.002641384,"teacher_disagreement_score":0.002456794,"about_ca_system_score_codex":0.00038807184,"about_ca_system_score_gemma":0.0001369837,"threshold_uncertainty_score":0.0068191886},"labels":[],"label_agreement":null},{"id":"W4353106540","doi":"10.3847/1538-4357/acb4eb","title":"Addressing Systematics in the Traceback Age of the β Pictoris Moving Group","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; myr; Parallax; Redshift; Kinematics; Astrophysics; Geology; Geodesy; Astronomy; Chemistry; Galaxy","score_opus":0.03824345546862556,"score_gpt":0.26394198026257953,"score_spread":0.22569852479395397,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4353106540","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96257854,0.00014573139,0.03459468,0.000052479314,0.00001958833,0.000015039677,0.0005635812,0.00049587386,0.001534385],"genre_scores_gemma":[0.9868737,0.00003900412,0.0120027615,0.000013461221,0.000011603004,0.000009331496,0.0006508187,0.000086010084,0.0003132711],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99951565,0.00011034387,0.00003327144,0.0001599706,0.00014238288,0.000038453953],"domain_scores_gemma":[0.99593985,0.0016190375,0.0008759147,0.0008232959,0.0006214356,0.000120443794],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017163875,0.00023808818,0.0002477546,0.0017679275,0.0003974415,0.00080621423,0.00055909535,0.00021883863,0.0013183614],"category_scores_gemma":[0.010820858,0.00014647709,0.00023716742,0.0012319115,0.00029368486,0.00049624237,0.0006674477,0.0002537235,0.00038211248],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000121256126,0.000016234722,0.89026904,0.000049344846,0.00008675517,0.00013759172,0.00070270314,0.014352798,0.0087177325,0.0015791773,0.000805876,0.083161615],"study_design_scores_gemma":[0.000022007885,0.000097540586,0.81396395,0.00005739214,0.00009414128,0.0004666965,0.0004536775,0.14615397,0.026343144,0.00482639,0.0074855895,0.000035397647],"about_ca_topic_score_codex":0.004034681,"about_ca_topic_score_gemma":0.0044319048,"teacher_disagreement_score":0.004034681,"about_ca_system_score_codex":0.00038540206,"about_ca_system_score_gemma":0.0002681779,"threshold_uncertainty_score":0.009077251},"labels":[],"label_agreement":null},{"id":"W4360613372","doi":"10.3847/1538-4357/acb432","title":"The Type Ibn Supernova 2019kbj: Indications for Diversity in Type Ibn Supernova Progenitors","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Astrophysics Science Division; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Council for Higher Education; Astrophysics Division; Canadian Institute for Advanced Research; United States-Israel Binational Science Foundation; European Research Council; Nuclear Safety and Security Commission; Space Telescope Science Institute; California Institute of Technology; National Aeronautics and Space Administration; Goddard Space Flight Center; Smithsonian Institution; National Science Foundation","keywords":"Physics; Ejecta; Supernova; Light curve; Astrophysics; Type (biology); Pair-instability supernova; Radioactive decay; Astronomy; Nuclear physics","score_opus":0.027568506528020977,"score_gpt":0.2682554302319612,"score_spread":0.2406869237039402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4360613372","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99774915,0.0002894305,0.00027326267,0.000012416043,0.0000046967825,0.0000036249266,0.00028216583,0.00001930745,0.0013659387],"genre_scores_gemma":[0.9991418,0.000071133625,0.00015369583,0.00000908097,0.0000028893974,0.0000023698165,0.0004437778,0.0000060547477,0.00016923383],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987626,0.000009294143,0.000016517894,0.000043571054,0.000025034333,0.000029212273],"domain_scores_gemma":[0.9993917,0.00008152184,0.00020641861,0.000061272396,0.000095622694,0.00016333432],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002497018,0.00023740114,0.000305229,0.00097500294,0.0003930312,0.0008762472,0.00027214605,0.0003145117,0.001590099],"category_scores_gemma":[0.00056393,0.00017096699,0.0002614674,0.00072617293,0.00023672212,0.00022845482,0.0005194247,0.00017496408,0.0004946775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032206663,0.00003067262,0.95895165,0.00003836049,0.000046981433,0.00060659554,0.00007932599,0.00047733777,0.034343377,0.00027426213,0.00014239595,0.0046870047],"study_design_scores_gemma":[0.000004280733,0.00003642035,0.99486816,0.000010213099,0.000021227745,0.0014463563,0.00012950625,0.0008623041,0.0015501408,0.00017928249,0.000885449,0.0000066357456],"about_ca_topic_score_codex":0.0028578492,"about_ca_topic_score_gemma":0.004037828,"teacher_disagreement_score":0.0028578492,"about_ca_system_score_codex":0.00032033186,"about_ca_system_score_gemma":0.00012304091,"threshold_uncertainty_score":0.0056824684},"labels":[],"label_agreement":null},{"id":"W4360620511","doi":"10.3847/1538-4357/acbb62","title":"On the Spectral Evolution of Hot White Dwarf Stars. IV. The Diffusion and Mixing of Residual Hydrogen in Helium-rich White Dwarfs","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"White dwarf; Physics; Astrophysics; Blue dwarf; Hydrogen; Black dwarf; Stellar evolution; Helium; Population; Stellar classification; Radiative transfer; Stars; Astronomy; Atomic physics","score_opus":0.010491431471308736,"score_gpt":0.21699940305973392,"score_spread":0.20650797158842518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4360620511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98657864,0.00009894372,0.009160359,0.00010918574,0.000007890283,0.000012811309,0.00014597407,0.00008783091,0.003798484],"genre_scores_gemma":[0.9981989,0.00004592916,0.0009073872,0.000017539352,0.0000039948213,0.000007759886,0.000054824308,0.000021191612,0.0007424235],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999347,0.00002384553,0.0000028380787,0.0000092474365,0.00001345947,0.000015849531],"domain_scores_gemma":[0.9996778,0.00015036979,0.00005506946,0.000036516416,0.000031725074,0.00004860039],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037600507,0.0004327154,0.0005319331,0.00036601478,0.0005282699,0.0006479489,0.00060842925,0.0007641962,0.0012514503],"category_scores_gemma":[0.0012483519,0.00026346958,0.0006429918,0.00023452635,0.0006014119,0.0006552503,0.0005432221,0.00038519985,0.00021944141],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000054148837,0.000043536336,0.008716939,0.000021586484,0.000024980365,0.00012974217,0.000054776938,0.9820128,0.0040498558,0.0035363666,0.00012797823,0.0012272876],"study_design_scores_gemma":[0.000018740815,0.000023709865,0.0023847462,0.0000024481576,0.000006697887,0.0000209172,0.000019877516,0.9953577,0.0009845515,0.0010317642,0.00014339657,0.0000053548615],"about_ca_topic_score_codex":0.012177981,"about_ca_topic_score_gemma":0.0046156696,"teacher_disagreement_score":0.012177981,"about_ca_system_score_codex":0.0010088158,"about_ca_system_score_gemma":0.00046043843,"threshold_uncertainty_score":0.024214208},"labels":[],"label_agreement":null},{"id":"W4361267400","doi":"10.3847/1538-4357/acdcf6","title":"The PAndAS View of the Andromeda Satellite System. IV. Global Properties","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Centre National de la Recherche Scientifique; Equipex; Agencia Estatal de Investigación; National Aeronautics and Space Administration; Agence Nationale de la Recherche; Space Telescope Science Institute; Ministerio de Ciencia e Innovación; Université de Strasbourg","keywords":"Physics; Andromeda; Satellite; Astronomy; Remote sensing; Astrophysics; Stars; Milky Way; Geography","score_opus":0.015622591654969289,"score_gpt":0.22313145830773337,"score_spread":0.20750886665276408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361267400","genre_codex":"other","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.060431868,0.008165,0.21135417,0.0074587604,0.00074801844,0.00014337266,0.08900231,0.054324735,0.5683718],"genre_scores_gemma":[0.6847645,0.0051594614,0.16515729,0.0011701606,0.0009460618,0.00016720878,0.054731257,0.0110802045,0.076823875],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"observational","domain_scores_codex":[0.99982256,0.000041513813,0.000007973442,0.00005872279,0.000049675582,0.000019559178],"domain_scores_gemma":[0.9996717,0.00007396663,0.000044440054,0.00012237034,0.000048372036,0.00003914325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004070596,0.00051351334,0.00028164554,0.0013931831,0.00048704538,0.002673694,0.0006470624,0.00041986138,0.029685441],"category_scores_gemma":[0.0008326739,0.0003598171,0.00052972353,0.001411457,0.0003990453,0.0024115029,0.000919849,0.0007001401,0.007234928],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004249929,0.000064958025,0.06388795,0.0007220464,0.00023722668,0.00087484147,0.0012861709,0.027649378,0.008915331,0.3361162,0.26182613,0.2979948],"study_design_scores_gemma":[0.000016998874,0.00001977614,0.025648188,0.00011945936,0.000043269727,0.00058046845,0.000289953,0.018721903,0.0011222967,0.032551225,0.9208491,0.000037374793],"about_ca_topic_score_codex":0.022592649,"about_ca_topic_score_gemma":0.03191368,"teacher_disagreement_score":0.029685441,"about_ca_system_score_codex":0.0005392614,"about_ca_system_score_gemma":0.00044073042,"threshold_uncertainty_score":0.09930766},"labels":[],"label_agreement":null},{"id":"W4361272321","doi":"10.3847/1538-4357/acbe39","title":"COOL–LAMPS. III. Discovery of a 25.″9 Separation Quasar Lensed by a Merging Galaxy Cluster*  ","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Los Alamos National Laboratory; Lawrence Berkeley National Laboratory; Argonne National Laboratory; Leibniz-Gemeinschaft; Science Mission Directorate; Turun Yliopisto; Smithsonian Astrophysical Observatory; University of Illinois at Urbana-Champaign; Eötvös Loránd Tudományegyetem; Max-Planck-Institut für Astrophysik; National Central University; Háskóli Íslands; University of Edinburgh; Queen's University; Integrated Electronics Engineering Center, Binghamton University; Johns Hopkins University; Universitetet i Oslo; High Energy Physics; Deutsche Forschungsgemeinschaft; Durham University; Office of Science; Fermilab; Max-Planck-Institut für Astronomie; University of Nottingham; Carnegie Institution for Science; Instituto de Astrofísica de Canarias; University of Cambridge; University of Chicago; National Energy Research Scientific Computing Center; University of Sussex; Space Telescope Science Institute; Stockholms Universitet; University of Utah; University of Portsmouth; National Aeronautics and Space Administration; University College London; Carnegie Mellon University; Alfred P. Sloan Foundation; Planetary Science Division; Carnegie Institution of Washington; Ohio State University; National Science Foundation; University of Michigan; U.S. Department of Energy; Smithsonian Institution; Division of Astronomical Sciences; Financiadora de Estudos e Projetos; University of Pennsylvania; Queen's University Belfast; Gordon and Betty Moore Foundation; Science and Technology Facilities Council; Aarhus Universitet","keywords":"Physics; ROSAT; Astrophysics; Quasar; Sky; Galaxy; Galaxy cluster; Cluster (spacecraft); Line-of-sight; Halo; Astronomy","score_opus":0.008364587905459629,"score_gpt":0.23655450078232057,"score_spread":0.22818991287686094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361272321","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9919775,0.00043086655,0.0010495725,0.0003313855,0.000025612848,0.000020395662,0.0009119214,0.00018812863,0.005064648],"genre_scores_gemma":[0.99500024,0.00009303468,0.001802679,0.00021175352,0.000050734256,0.000010405314,0.00092879136,0.000024813327,0.0018775105],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976224,0.00001649355,0.000009416087,0.00008290294,0.000066271896,0.00006266496],"domain_scores_gemma":[0.999348,0.00005551503,0.00022825002,0.00006433951,0.0000590862,0.00024474884],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004652805,0.00029304324,0.00023845416,0.0015559907,0.000961396,0.0009297432,0.00031240875,0.00052373327,0.002099585],"category_scores_gemma":[0.0004323178,0.00027247888,0.00039209618,0.00057504047,0.00049763406,0.00033897717,0.0009477721,0.00034017224,0.00048524624],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011648585,0.00011715915,0.75700736,0.00017802714,0.00023635202,0.018043134,0.0029545382,0.00027620018,0.15567496,0.0027139531,0.010000066,0.05163345],"study_design_scores_gemma":[0.00004370804,0.00035311276,0.9225494,0.000032932363,0.00012218131,0.012240479,0.0007015179,0.00071385654,0.028358595,0.0006861903,0.034146324,0.000051617535],"about_ca_topic_score_codex":0.003260047,"about_ca_topic_score_gemma":0.004846626,"teacher_disagreement_score":0.003260047,"about_ca_system_score_codex":0.00052315474,"about_ca_system_score_gemma":0.00018632505,"threshold_uncertainty_score":0.0070237517},"labels":[],"label_agreement":null},{"id":"W4361272525","doi":"10.3847/1538-4357/acbbd0","title":"An FRB Sent Me a DM: Constraining the Electron Column of the Milky Way Halo with Fast Radio Burst Dispersion Measures from CHIME/FRB","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":67,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; Perimeter Institute; University of British Columbia; University of Toronto; Ontario Power Generation; McGill University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics","funders":"Division of Astronomical Sciences; Division of Physics; Natural Sciences and Engineering Research Council of Canada; Canada Foundation for Innovation","keywords":"Physics; Halo; Milky Way; Astrophysics; Galactic halo; Galaxy; Fast radio burst; Population; Astronomy; Velocity dispersion","score_opus":0.007743146320803199,"score_gpt":0.20474074428640454,"score_spread":0.19699759796560135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361272525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99431413,0.0006102738,0.0026163636,0.00008432784,0.0000065643435,0.0000045348056,0.0008845944,0.00012536098,0.0013538676],"genre_scores_gemma":[0.9976236,0.00009061229,0.0012198708,0.000019852572,0.000009767218,0.0000028039542,0.00088663003,0.000025459163,0.00012130052],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985874,0.00003217685,0.0000057464563,0.000040338033,0.00003233589,0.000030723517],"domain_scores_gemma":[0.99920183,0.00020434083,0.0002032098,0.00013692223,0.000093818155,0.00015987126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076379837,0.00040377976,0.00024635778,0.0011509757,0.00020170011,0.00082105753,0.00033765865,0.0002647674,0.00074568676],"category_scores_gemma":[0.0013800767,0.00023795041,0.0003980793,0.0007509986,0.00019748513,0.00024267669,0.0007256666,0.00022582422,0.00022554577],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000338708,0.000033105385,0.93602604,0.0000964369,0.00046378176,0.00026469803,0.00018203346,0.017482668,0.023532597,0.0011066204,0.0011764935,0.019296778],"study_design_scores_gemma":[0.00003520617,0.00003412537,0.9628686,0.000036983787,0.00009651438,0.00008919653,0.000092447255,0.029457705,0.004481082,0.0005404503,0.0022413435,0.000026478097],"about_ca_topic_score_codex":0.011706231,"about_ca_topic_score_gemma":0.010661218,"teacher_disagreement_score":0.011706231,"about_ca_system_score_codex":0.00034902492,"about_ca_system_score_gemma":0.00017760605,"threshold_uncertainty_score":0.02327621},"labels":[],"label_agreement":null},{"id":"W4361272725","doi":"10.3847/1538-4357/acbea4","title":"First BISTRO Observations of the Dark Cloud Taurus L1495A-B10: The Role of the Magnetic Field in the Earliest Stages of Low-mass Star Formation","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; McMaster University; Queen's University; University of Manitoba; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Agencia Estatal de Investigación; Science and Engineering Research Board; Japan Society for the Promotion of Science; National Research Foundation; Science and Technology Facilities Council; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; National Research Foundation of Korea; Academia Sinica; Department of Science and Technology, Ministry of Science and Technology, India; Canadian Space Agency; National Science Foundation; Royal Society; Korea Astronomy and Space Science Institute","keywords":"Physics; Astrophysics; Magnetic field; Molecular cloud; Star formation; Protein filament; James Clerk Maxwell Telescope; Sky; Polarization (electrochemistry); Stars; Materials science","score_opus":0.011496324174640216,"score_gpt":0.2188997510530217,"score_spread":0.20740342687838148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4361272725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980393,0.00005896922,0.00027449572,0.000030046263,0.0000029170938,0.0000039731426,0.00017934952,0.0000144014175,0.0013964558],"genre_scores_gemma":[0.999559,0.000013184459,0.00012585637,0.000013082268,0.0000027183394,0.0000016935905,0.00015087676,0.0000016844881,0.00013191797],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995935,0.0000038805547,0.000001619051,0.000009695251,0.000010040293,0.000015341848],"domain_scores_gemma":[0.9998405,0.000016776869,0.000033829176,0.000015612935,0.000027284315,0.00006590282],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000104986146,0.00012664305,0.00010455296,0.00031472108,0.00030654043,0.0003551338,0.00020873296,0.00029786077,0.00079084357],"category_scores_gemma":[0.00026101954,0.00009739696,0.00009439336,0.00011653756,0.00016421756,0.00021043375,0.00030111172,0.00021309976,0.00022003958],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039233838,0.00008133887,0.7672802,0.000026281374,0.000037668484,0.0003609272,0.00020202667,0.00028496646,0.22203888,0.00031078578,0.00036758668,0.008616883],"study_design_scores_gemma":[0.0000058013925,0.00005496067,0.9952834,0.0000038597645,0.0000062401214,0.00007984309,0.00006181716,0.0004605203,0.003533785,0.000040104194,0.00046669212,0.0000028994418],"about_ca_topic_score_codex":0.0035754677,"about_ca_topic_score_gemma":0.008384682,"teacher_disagreement_score":0.0035754677,"about_ca_system_score_codex":0.000288102,"about_ca_system_score_gemma":0.00005678702,"threshold_uncertainty_score":0.007109344},"labels":[],"label_agreement":null},{"id":"W4362474209","doi":"10.3847/1538-4357/acba87","title":"Stellar Initial Mass Function (IMF) Probed with Supernova Rates and Neutrino Background: Cosmic-average IMF Slope Is ≃2–3 Similar to the Salpeter IMF","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Astronomical Observatory of Japan; University of Tokyo; Institute for Cosmic Ray Research, University of Tokyo; Ministry of Education, Culture, Sports, Science and Technology; Japan Society for the Promotion of Science; Canadian Foundation for Climate and Atmospheric Sciences","keywords":"Physics; Supernova; Initial mass function; Astrophysics; Neutrino; Galaxy; COSMIC cancer database; Star formation; Redshift; Stars; Astronomy","score_opus":0.01796797975393977,"score_gpt":0.24486265395395734,"score_spread":0.22689467420001758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362474209","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99747735,0.000103032085,0.0007507702,0.000015510292,0.0000019028316,0.0000021397968,0.0005127631,0.000052367912,0.0010841724],"genre_scores_gemma":[0.9990139,0.000022187149,0.00026989813,0.000005555861,0.0000027509907,0.0000011548634,0.00058624655,0.0000061717046,0.00009213857],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998497,0.000027393446,0.000008668723,0.000057594374,0.000024773984,0.000031803178],"domain_scores_gemma":[0.99935335,0.00012468551,0.00025415083,0.00009108087,0.000084262865,0.00009259939],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052590505,0.00031891948,0.00020376785,0.0006969828,0.00013103492,0.00045320299,0.00017516255,0.00021880961,0.0015334309],"category_scores_gemma":[0.0009952651,0.00012406828,0.00023998527,0.00048878783,0.00016304766,0.0002761147,0.00032488123,0.0001734477,0.00031794075],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000103187616,0.000008793979,0.98749334,0.0000073104115,0.00004932442,0.000039121664,0.000028969325,0.0005218364,0.008667486,0.00010346017,0.0000683965,0.0029087202],"study_design_scores_gemma":[0.0000013553008,0.000014470127,0.99665713,0.0000026779453,0.000013361803,0.000095068295,0.000021312004,0.0012551559,0.0017332586,0.000059615693,0.000144201,0.0000024114302],"about_ca_topic_score_codex":0.0015297418,"about_ca_topic_score_gemma":0.0018122775,"teacher_disagreement_score":0.0015334309,"about_ca_system_score_codex":0.00015349008,"about_ca_system_score_gemma":0.000064003216,"threshold_uncertainty_score":0.005129814},"labels":[],"label_agreement":null},{"id":"W4362554345","doi":"10.3847/1538-4357/acc4bf","title":"Tracking the Enigmatic Globular Cluster Ultracompact X-Ray Binary X1850–087: Extreme Radio Variability in the Hard State","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Division of Graduate Education; RIKEN; Nuclear Safety and Security Commission; Japan Aerospace Exploration Agency; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Jansky; Ejecta; Neutron star; Globular cluster; Astronomy; Spectral index; Black hole (networking); X-ray binary; Synchrotron; Luminosity; Supernova; Binary number; Stars; Galaxy; Radio galaxy; Spectral line","score_opus":0.03120440718978134,"score_gpt":0.252943786161191,"score_spread":0.22173937897140966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362554345","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99960035,0.000013119906,0.00005436318,0.00000466104,6.59771e-7,0.0000013530291,0.000030955005,0.0000027856559,0.00029168875],"genre_scores_gemma":[0.9994504,0.000010489437,0.00018448068,0.0000066315797,0.0000021152973,0.0000023300736,0.00017958904,0.0000019478298,0.00016190515],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995196,0.000005128962,0.0000014551695,0.0000124349135,0.000012274207,0.000016758044],"domain_scores_gemma":[0.99986815,0.000013036279,0.00003768821,0.000014329243,0.000018964362,0.000047897844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016796669,0.00008519852,0.00014195513,0.000282616,0.0002974144,0.00036689182,0.00019071513,0.0001410464,0.0004633112],"category_scores_gemma":[0.0001825848,0.00006134202,0.000062178675,0.00016260937,0.00023219017,0.00011440382,0.00046981304,0.00014208852,0.00019186072],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020397895,0.00009420587,0.9477287,0.000014132234,0.000037596357,0.0002694567,0.000407284,0.00030874307,0.043461792,0.00024390627,0.00029422113,0.0069359755],"study_design_scores_gemma":[0.0000034830427,0.000069167414,0.9977118,0.0000019575848,0.0000073009414,0.000089951616,0.00016658756,0.0004692506,0.0009914052,0.000035550016,0.0004515933,0.000001965689],"about_ca_topic_score_codex":0.0030299316,"about_ca_topic_score_gemma":0.008277018,"teacher_disagreement_score":0.0030299316,"about_ca_system_score_codex":0.00018882769,"about_ca_system_score_gemma":0.00010651496,"threshold_uncertainty_score":0.006024599},"labels":[],"label_agreement":null},{"id":"W4362581663","doi":"10.3847/1538-4357/acbf36","title":"Search for a Black Hole Binary in Gaia DR3 Astrometric Binary Stars with Spectroscopic Data","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Neutron star; Primary (astronomy); Astronomy; Binary number; Binary system; Red giant; Stars; Binary star; Mass ratio; Orbital elements; X-ray binary; Compact star; Orbital period; Black hole (networking)","score_opus":0.044988040651890555,"score_gpt":0.29594462704797125,"score_spread":0.2509565863960807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362581663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979202,0.00013378196,0.00037903566,0.000043261745,0.0000066728185,0.000009321934,0.00020407738,0.000024034784,0.0012795827],"genre_scores_gemma":[0.9987178,0.00002194314,0.00068944244,0.000024175812,0.0000038083124,0.0000031201932,0.00035228292,0.0000032619796,0.00018412093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980396,0.000023528577,0.000014816604,0.000052224026,0.000059868977,0.00004571842],"domain_scores_gemma":[0.99938273,0.00006819487,0.0002694314,0.00006963028,0.00008016446,0.00012977734],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034608002,0.00022662272,0.0003026068,0.0015744172,0.0007233132,0.0005256575,0.00033039862,0.0004617568,0.001031767],"category_scores_gemma":[0.0006076533,0.00014107398,0.0003198305,0.0013165853,0.000258952,0.00020715791,0.000601591,0.00026988797,0.0005308651],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021892125,0.000060980365,0.9526277,0.000041309177,0.00005720572,0.0012297198,0.0003595712,0.00026581893,0.03235496,0.0004367686,0.00040903658,0.011938046],"study_design_scores_gemma":[0.000017001948,0.00019448034,0.9850176,0.000013810983,0.00006027076,0.0024081198,0.0004483118,0.0024749688,0.0054792017,0.00030034358,0.003570584,0.000015251758],"about_ca_topic_score_codex":0.003447624,"about_ca_topic_score_gemma":0.005780252,"teacher_disagreement_score":0.003447624,"about_ca_system_score_codex":0.00041303292,"about_ca_system_score_gemma":0.00032777706,"threshold_uncertainty_score":0.00685513},"labels":[],"label_agreement":null},{"id":"W4362583683","doi":"10.3847/1538-4357/acbea0","title":"A Search for Coincident Neutrino Emission from Fast Radio Bursts with Seven Years of IceCube Cascade Events","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; National Research Foundation; Michigan State University; University of Oxford; Compute Canada; Marquette University","keywords":"Physics; Neutrino; Astrophysics; Astronomy; Cascade; Neutrino astronomy; Event (particle physics); Observatory; Range (aeronautics); Flux (metallurgy); Neutrino detector; Neutrino oscillation; Nuclear physics","score_opus":0.012728807200172554,"score_gpt":0.2509746650497658,"score_spread":0.23824585784959323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362583683","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974722,0.000110122484,0.00046432897,0.000016511876,0.0000059104773,0.000019951152,0.0004936317,0.000020657113,0.0013967224],"genre_scores_gemma":[0.99621236,0.000070980954,0.0012286213,0.00003078587,0.000019332576,0.000019415906,0.0021005096,0.000014504418,0.00030338616],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993381,0.00008807761,0.000030533505,0.0002136971,0.00018231476,0.00014733158],"domain_scores_gemma":[0.9978047,0.0006178371,0.00085660396,0.00015374945,0.00022322165,0.00034383585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00084100803,0.00036279354,0.000369958,0.0017226,0.0005335914,0.000876582,0.0003489875,0.00047966972,0.0017064444],"category_scores_gemma":[0.0015333651,0.00021148089,0.0004000001,0.0013086835,0.0002679052,0.0002732083,0.0007087539,0.0002969231,0.00023862677],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016729548,0.00022427295,0.9253882,0.000053667736,0.00024552082,0.0013638863,0.00033141836,0.0006076352,0.057695672,0.00034242854,0.0004652737,0.011609009],"study_design_scores_gemma":[0.000040193605,0.00040059193,0.98574674,0.000013174044,0.000100873796,0.0010914357,0.00023624784,0.0009161826,0.0092503065,0.000082946455,0.0021055418,0.000015767131],"about_ca_topic_score_codex":0.0034374604,"about_ca_topic_score_gemma":0.0052695307,"teacher_disagreement_score":0.0034374604,"about_ca_system_score_codex":0.0004573098,"about_ca_system_score_gemma":0.0004229679,"threshold_uncertainty_score":0.006834924},"labels":[],"label_agreement":null},{"id":"W4362589080","doi":"10.3847/1538-4357/acbfaa","title":"Distillation of <sup>56</sup>Fe in Ultramassive O–Ne White Dwarfs","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Office of International Science and Engineering; Division of Physics","keywords":"White dwarf; Physics; Astrophysics; Supernova; Nucleosynthesis; Asteroseismology; Stars","score_opus":0.008722775054271539,"score_gpt":0.22143390004369487,"score_spread":0.21271112498942332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362589080","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989002,0.000023846249,0.0006735457,0.000008596266,0.0000013595043,0.0000014317862,0.000031157033,0.000020021638,0.00033981225],"genre_scores_gemma":[0.999438,0.000010099249,0.0003013146,0.0000038108333,6.201254e-7,0.0000011954667,0.000054531607,0.000008191759,0.00018211419],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99996674,0.000003763325,0.0000021857174,0.000008762211,0.000009587706,0.000009045716],"domain_scores_gemma":[0.9998889,0.000038093778,0.000028827842,0.000009567697,0.000013316207,0.00002119935],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013283695,0.00018059208,0.0002070886,0.00023908797,0.00021216353,0.0003194103,0.00025594712,0.0002081709,0.0008244613],"category_scores_gemma":[0.0003086042,0.00012289188,0.00019292452,0.00011297144,0.0002675866,0.00026707636,0.00026048205,0.00020224202,0.0001416706],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010912928,0.00013937076,0.095638424,0.00011421157,0.00008852813,0.0007895756,0.00025741226,0.120248295,0.76506674,0.003876792,0.00029099683,0.012398247],"study_design_scores_gemma":[0.00009547618,0.00042280217,0.10668618,0.000008864125,0.00003234558,0.00031878098,0.00017854215,0.44221187,0.44578713,0.0023692874,0.0018478883,0.00004079598],"about_ca_topic_score_codex":0.0036445078,"about_ca_topic_score_gemma":0.0033906547,"teacher_disagreement_score":0.0036445078,"about_ca_system_score_codex":0.00044325186,"about_ca_system_score_gemma":0.00011587425,"threshold_uncertainty_score":0.007246554},"labels":[],"label_agreement":null},{"id":"W4362600417","doi":"10.3847/1538-4357/acbf4b","title":"The Halo Mass–Temperature Relation for Clusters, Groups, and Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"","keywords":"Astrophysics; Physics; Halo; Galaxy; Galaxy cluster; RADIUS; Hydrostatic equilibrium; Power law; Cluster (spacecraft); Elliptical galaxy; Galaxy groups and clusters; Astronomy; Statistics","score_opus":0.006680102962958079,"score_gpt":0.20937033356359294,"score_spread":0.20269023060063487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362600417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99678457,0.00034965988,0.00073949154,0.000023384413,0.000003158013,0.000005083006,0.00047529917,0.000038066813,0.0015811977],"genre_scores_gemma":[0.9993193,0.000037771948,0.00026162082,0.000005463712,0.0000036183255,0.0000021333774,0.0002476636,0.0000041106478,0.00011847114],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979705,0.00003073287,0.000016942031,0.00006771599,0.00004602033,0.00004158808],"domain_scores_gemma":[0.9975973,0.0005736952,0.0008581948,0.00034684342,0.00033302297,0.00029107952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044916235,0.00018757355,0.00018211447,0.0017785176,0.0002876738,0.0004725386,0.00020328407,0.00017189152,0.0015468274],"category_scores_gemma":[0.0029239126,0.00012153737,0.00022709445,0.00093017385,0.0003108724,0.00034685706,0.00047540796,0.00016247857,0.00046916184],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008099614,0.000008468977,0.9887279,0.000018729423,0.000070625676,0.00004205801,0.00016293312,0.0013086903,0.0036553792,0.00045741507,0.00031620555,0.005150479],"study_design_scores_gemma":[0.000002679345,0.000030129673,0.9960461,0.00000404542,0.00001789525,0.00018072787,0.00005873326,0.0017353905,0.00095303456,0.00036374186,0.00060188014,0.0000054769416],"about_ca_topic_score_codex":0.003128228,"about_ca_topic_score_gemma":0.003190103,"teacher_disagreement_score":0.003128228,"about_ca_system_score_codex":0.00033595046,"about_ca_system_score_gemma":0.00011978233,"threshold_uncertainty_score":0.0062200427},"labels":[],"label_agreement":null},{"id":"W4362737852","doi":"10.3847/1538-4357/acbf44","title":"AGN STORM 2. III. A NICER View of the Variable X-Ray Obscurer in Mrk 817","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Astrophysics Science Division; Goddard Space Flight Center; Alexander von Humboldt-Stiftung; National Aeronautics and Space Administration; Chinese Academy of Sciences; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; X-ray; Nuclear physics","score_opus":0.014768362318399808,"score_gpt":0.23561562117607251,"score_spread":0.2208472588576727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4362737852","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97299206,0.00060284225,0.0009945977,0.00081733754,0.00003479302,0.000016866994,0.0029699758,0.0005259041,0.021045716],"genre_scores_gemma":[0.9861296,0.00018966258,0.0021653064,0.00052906695,0.00012686737,0.000013069992,0.005158783,0.00022303194,0.0054647215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999027,0.0000064445094,0.000003823084,0.000025477471,0.000027311788,0.00003426398],"domain_scores_gemma":[0.99977094,0.000023082546,0.00008020293,0.000036886013,0.000024102977,0.0000647563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016892781,0.00018914827,0.00028170057,0.0011160674,0.00054422754,0.0008128308,0.0003428274,0.00040929034,0.002497445],"category_scores_gemma":[0.00018857258,0.00017800988,0.0003267328,0.00045456714,0.00024841927,0.0003642647,0.00077282684,0.00054001727,0.0011252788],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012029505,0.00016446652,0.5748716,0.00031281865,0.00015279258,0.023483299,0.0035821851,0.0036650922,0.26588458,0.0066181,0.054668628,0.065393485],"study_design_scores_gemma":[0.000038465576,0.000073702875,0.9581734,0.00003521159,0.000030004772,0.0038097252,0.000608391,0.0034405598,0.004435088,0.0011750587,0.028145751,0.00003468325],"about_ca_topic_score_codex":0.0056451545,"about_ca_topic_score_gemma":0.010005849,"teacher_disagreement_score":0.0056451545,"about_ca_system_score_codex":0.00055719295,"about_ca_system_score_gemma":0.00015972159,"threshold_uncertainty_score":0.011224568},"labels":[],"label_agreement":null},{"id":"W4365141570","doi":"10.3847/1538-4357/acbbca","title":"SDSS-IV MaNGA: The Effect of Stellar Mass and Halo Mass on the Assembly Histories of Satellite Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; University of Oxford; Universidad de Atacama; Ministério da Ciência, Tecnologia e Inovação; Vanderbilt University; Consejo Nacional de Ciencia y Tecnología; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Chinese University of Hong Kong; University of California, Santa Cruz; Faculty of Science, Chinese University of Hong Kong; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Yale University","keywords":"Physics; Satellite galaxy; Galaxy; Astrophysics; Halo; Stellar mass; Astronomy; Satellite; Sky; RADIUS; Star formation","score_opus":0.0072864282537013535,"score_gpt":0.20797068527626753,"score_spread":0.20068425702256618,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4365141570","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973328,0.00022309927,0.00024699763,0.00007327546,0.0000060351226,0.0000034345076,0.0015133945,0.00007645443,0.0005243923],"genre_scores_gemma":[0.998382,0.000024920322,0.00020933375,0.00002032611,0.00000668399,0.000003566903,0.0011562003,0.000044272176,0.00015280057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990421,0.00038190346,0.000044478908,0.00029955726,0.000111770285,0.00012026933],"domain_scores_gemma":[0.9937145,0.0022221634,0.001523999,0.0011473157,0.0003677762,0.0010241482],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027604261,0.00029694632,0.0004935109,0.0014176125,0.0005552738,0.001063404,0.0004208999,0.00022187646,0.0013091374],"category_scores_gemma":[0.0043513034,0.0002661148,0.0005957156,0.001125987,0.0005535202,0.0005838286,0.00086095685,0.00030624922,0.0004914283],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000095835705,0.000010690874,0.9947147,0.000010736628,0.00015102184,0.00003445262,0.000090172725,0.0004207135,0.0025858006,0.0000626849,0.00030641994,0.0015168417],"study_design_scores_gemma":[0.0000019969934,0.0000132090745,0.9983375,0.0000029440814,0.000021671382,0.000021031983,0.000051357958,0.0010538276,0.000265846,0.000030458255,0.0001965735,0.0000034523384],"about_ca_topic_score_codex":0.008781263,"about_ca_topic_score_gemma":0.013875558,"teacher_disagreement_score":0.008781263,"about_ca_system_score_codex":0.00036811733,"about_ca_system_score_gemma":0.00024299294,"threshold_uncertainty_score":0.017460287},"labels":[],"label_agreement":null},{"id":"W4365144517","doi":"10.3847/1538-4357/acb13f","title":"Detection of Cosmological 21 cm Emission with the Canadian Hydrogen Intensity Mapping Experiment","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":85,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Okanagan University College; Perimeter Institute; University of British Columbia, Okanagan Campus; Herzberg Institute of Astrophysics; Thompson Rivers University; McGill University; University of British Columbia","funders":"Office of Science; National Research Council Canada; University of Toronto; Industry Canada; Canada Foundation for Innovation; National Science Foundation; Compute Canada; University of Utah; Smithsonian Astrophysical Observatory; Western Canada Research Grid; Canadian Institute for Advanced Research; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Alfred P. Sloan Foundation; McGill University; U.S. Department of Energy; Government of Canada","keywords":"Physics; Astrophysics; Redshift; Galaxy; Intensity mapping; Omega; Reionization; Quasar; Emission spectrum; Spectral line; Astronomy; Quantum mechanics","score_opus":0.017170905590606904,"score_gpt":0.22007618737302687,"score_spread":0.20290528178241996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4365144517","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9789534,0.00020086317,0.001762215,0.0003819116,0.0000125794995,0.000033805012,0.004203545,0.000101990634,0.014349652],"genre_scores_gemma":[0.9951597,0.00007328572,0.0017370859,0.00009854443,0.000008862149,0.000014523207,0.0018032783,0.000015461435,0.0010892312],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993975,0.00004470297,0.0000092067685,0.00010886411,0.00027198475,0.00016771571],"domain_scores_gemma":[0.9981487,0.00019174659,0.0003735239,0.00022693835,0.0006093729,0.00044977613],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007080744,0.00024044218,0.00017924985,0.0013876428,0.001413892,0.0005447496,0.00053791684,0.0002590335,0.0017826953],"category_scores_gemma":[0.002099885,0.00015069409,0.00015823467,0.0017474723,0.0005191388,0.00018785633,0.0007994827,0.00031436782,0.00020439344],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031537548,0.00005887774,0.91922826,0.0000532582,0.00009751651,0.0005594999,0.0011260324,0.0008540834,0.028818144,0.0034343002,0.009104056,0.036350526],"study_design_scores_gemma":[0.000004867405,0.000009410513,0.9929428,0.000005918733,0.000010015223,0.00008077618,0.000099092766,0.00037204378,0.001689522,0.00014901669,0.0046229702,0.00001365763],"about_ca_topic_score_codex":0.66530097,"about_ca_topic_score_gemma":0.83465225,"teacher_disagreement_score":0.66530097,"about_ca_system_score_codex":0.0039314018,"about_ca_system_score_gemma":0.0026700574,"threshold_uncertainty_score":0.67334026},"labels":[],"label_agreement":null},{"id":"W4365211514","doi":"10.3847/1538-4357/acfe06","title":"The Atacama Cosmology Telescope: A Measurement of the DR6 CMB Lensing Power Spectrum and Its Implications for Structure Growth","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":249,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McGill University; University of British Columbia; University of Toronto; Perimeter Institute","funders":"High Energy Physics; Japan Society for the Promotion of Science; Office of Science; National Institute of Standards and Technology; Agencia Nacional de Investigación y Desarrollo; Cambridge Trust; Industry Canada; University of Toronto; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; National Research Foundation; U.S. Department of Energy; European Commission; National Energy Research Scientific Computing Center; National Science Foundation; Compute Canada; National Aeronautics and Space Administration; Lawrence Berkeley National Laboratory; University of Pennsylvania; Ministry of Education, Culture, Sports, Science and Technology; Alfred P. Sloan Foundation; Princeton University; Institut Périmètre de physique théorique; Government of Ontario; Ministry of Colleges and Universities; Government of Canada","keywords":"Physics; Cosmic microwave background; Astrophysics; Cosmology; Astronomy; Spectral density; Telescope; Weak gravitational lensing; Galaxy; Redshift; Optics; Anisotropy","score_opus":0.016538293257792755,"score_gpt":0.2740965725320958,"score_spread":0.257558279274303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4365211514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9643925,0.00024610065,0.008122179,0.00039946596,0.000030534,0.000026655965,0.010912422,0.0003672916,0.015502847],"genre_scores_gemma":[0.9859599,0.000078207435,0.007763469,0.00005710881,0.000051582094,0.000016094029,0.0050991434,0.00010737107,0.0008670093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99896824,0.00016282166,0.00004411209,0.00023422448,0.0005339012,0.00005674204],"domain_scores_gemma":[0.9960672,0.0007458686,0.0012042685,0.0008466521,0.00069005357,0.00044598774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001391786,0.00039900898,0.00021435058,0.0017652686,0.00044393115,0.0007931031,0.00053061295,0.00034930103,0.00278788],"category_scores_gemma":[0.004921558,0.00029164966,0.00034782497,0.0019237376,0.0004250876,0.00066111627,0.00089363597,0.0006616962,0.00084363134],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003724899,0.00012602223,0.8888642,0.00011431802,0.00023570293,0.00033409082,0.0006146606,0.006953791,0.04386822,0.006668789,0.00926956,0.042578094],"study_design_scores_gemma":[0.000011062969,0.000021983555,0.9833218,0.000009437821,0.0000152181565,0.0001572703,0.000057174504,0.006497822,0.0046979166,0.0009528408,0.004240243,0.000017180937],"about_ca_topic_score_codex":0.006072144,"about_ca_topic_score_gemma":0.0065396433,"teacher_disagreement_score":0.006072144,"about_ca_system_score_codex":0.0005806128,"about_ca_system_score_gemma":0.00018630408,"threshold_uncertainty_score":0.012073576},"labels":[],"label_agreement":null},{"id":"W4365211529","doi":"10.3847/1538-4357/acff5f","title":"The Atacama Cosmology Telescope: DR6 Gravitational Lensing Map and Cosmological Parameters","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":307,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McGill University; University of British Columbia; University of Toronto; Perimeter Institute","funders":"Japan Society for the Promotion of Science; Office of Science; National Institute of Standards and Technology; Agencia Nacional de Investigación y Desarrollo; Industry Canada; University of Toronto; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; National Research Foundation; U.S. Department of Energy; European Commission; National Energy Research Scientific Computing Center; National Science Foundation; Compute Canada; National Aeronautics and Space Administration; Lawrence Berkeley National Laboratory; University of Pennsylvania; Ministry of Education, Culture, Sports, Science and Technology; Alfred P. Sloan Foundation; Princeton University; Institut Périmètre de physique théorique; Government of Ontario; Ministry of Colleges and Universities; Government of Canada","keywords":"Physics; Cosmology; Gravitational lens; Astrophysics; Strong gravitational lensing; Astronomy; Gravitation; Weak gravitational lensing; Gravitational lensing formalism; Telescope; Galaxy; Redshift","score_opus":0.01151407759395567,"score_gpt":0.2596380022138657,"score_spread":0.24812392461991,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4365211529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8535253,0.0012529613,0.0077871257,0.0016322734,0.00008583591,0.00003880087,0.055197395,0.0013867617,0.07909355],"genre_scores_gemma":[0.9562661,0.00026858662,0.0069032283,0.000162657,0.00009690478,0.000018734629,0.02821784,0.00026808042,0.007797837],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974316,0.00004376714,0.000008655384,0.00007926331,0.00008949569,0.00003560429],"domain_scores_gemma":[0.9991036,0.00011984987,0.00016494814,0.00015492814,0.00031097664,0.00014565651],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005781171,0.0003631112,0.00031864992,0.0014248786,0.00052696886,0.0008750157,0.00042461674,0.00039902682,0.011287739],"category_scores_gemma":[0.0017334587,0.00022351608,0.00030889595,0.001922372,0.00020503817,0.00048714664,0.00054313615,0.0004114123,0.0032439942],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009900575,0.00017250983,0.67245114,0.00043217602,0.00048554543,0.0009796849,0.00074311876,0.05195979,0.028335866,0.03163249,0.10763704,0.104180634],"study_design_scores_gemma":[0.000046250872,0.00003322185,0.9327889,0.000042389034,0.000053656455,0.00019681259,0.00014773596,0.026341805,0.0025287631,0.0040445374,0.033724915,0.00005087242],"about_ca_topic_score_codex":0.045862634,"about_ca_topic_score_gemma":0.030522175,"teacher_disagreement_score":0.045862634,"about_ca_system_score_codex":0.00089413935,"about_ca_system_score_gemma":0.00043372202,"threshold_uncertainty_score":0.09119141},"labels":[],"label_agreement":null},{"id":"W4365512778","doi":"10.3847/1538-4357/acbe3a","title":"Saying Hallo to M94's Stellar Halo: Investigating the Accretion History of the Largest Pseudobulge Host in the Local Universe","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Fondo Nacional de Desarrollo Científico y Tecnológico; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Agencia Nacional de Investigación y Desarrollo; National Central University; Max-Planck-Gesellschaft; Space Telescope Science Institute; National Science Foundation; University of Washington; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Durham University; Smithsonian Institution","keywords":"Halo; Astrophysics; Host (biology); Accretion (finance); Astronomy; Physics; Galaxy; Biology; Ecology","score_opus":0.013842903263880773,"score_gpt":0.20838586334819081,"score_spread":0.19454296008431005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4365512778","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993499,0.000036633264,0.000023305092,0.00002154487,7.797839e-7,0.0000011577445,0.00003600377,0.0000034862671,0.00052713207],"genre_scores_gemma":[0.99966645,0.000032743785,0.0000756741,0.000016430069,0.0000035463795,8.819457e-7,0.000047338843,0.0000025321783,0.00015440225],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994147,0.0000105023,0.000002767601,0.000011887756,0.00001273779,0.000020689102],"domain_scores_gemma":[0.9996567,0.000044474196,0.00010416773,0.000034967168,0.000048645317,0.00011110139],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022502273,0.00008640731,0.00012192913,0.0009869115,0.00077946484,0.000793779,0.00021780447,0.0001911907,0.001319612],"category_scores_gemma":[0.00061822974,0.000070592265,0.00009163047,0.00057429005,0.00031721743,0.00041564472,0.0007264073,0.00017026695,0.00024191616],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009333668,0.000020860476,0.985207,0.000013573434,0.000015971846,0.00037674492,0.0014307101,0.00005337828,0.0052064657,0.00020718887,0.00025030103,0.007124543],"study_design_scores_gemma":[0.0000012928313,0.000025389398,0.99670756,0.00000418964,0.000006785189,0.0001843689,0.0016163184,0.00010613801,0.00058705744,0.000062001396,0.0006961282,0.0000027905642],"about_ca_topic_score_codex":0.0052474965,"about_ca_topic_score_gemma":0.010023369,"teacher_disagreement_score":0.0052474965,"about_ca_system_score_codex":0.00037998162,"about_ca_system_score_gemma":0.0001119533,"threshold_uncertainty_score":0.010433912},"labels":[],"label_agreement":null},{"id":"W4365513212","doi":"10.3847/1538-4357/acb690","title":"Strong Variability in AzV 493, an Extreme Oe-type Star in the SMC","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Photosphere; Photometry (optics); Spectral line; Stars; Astronomy","score_opus":0.035465446871886276,"score_gpt":0.2627974536428571,"score_spread":0.22733200677097085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4365513212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982095,0.00008178339,0.00018217643,0.000021617949,0.0000035800706,0.0000016634813,0.00036701042,0.000019907413,0.0011128074],"genre_scores_gemma":[0.99903095,0.000023945338,0.00010541849,0.000015897262,0.000007816414,0.0000014581253,0.00063296175,0.0000062743966,0.00017525612],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999254,0.0000060904795,0.00000472249,0.000024173993,0.000018295877,0.000021307895],"domain_scores_gemma":[0.9998429,0.0000171912,0.000045019875,0.000018745344,0.000020720156,0.00005536367],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016289942,0.00016092439,0.00026117786,0.0005433037,0.00039526232,0.0005529193,0.00015917244,0.00023450734,0.00095406466],"category_scores_gemma":[0.00026134204,0.000072244286,0.00020742652,0.00037953287,0.0001958791,0.0001546315,0.00042752546,0.00018372359,0.0004883852],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029049005,0.000053349893,0.8992058,0.00002140776,0.00006968378,0.0006382592,0.00018658716,0.00056339824,0.08782329,0.00019359024,0.00060819427,0.010345999],"study_design_scores_gemma":[0.0000042990614,0.000027285834,0.99673814,0.0000023714563,0.000012559786,0.0001216651,0.000035713198,0.00059602945,0.001445875,0.00003774786,0.0009755487,0.0000028458967],"about_ca_topic_score_codex":0.0044876817,"about_ca_topic_score_gemma":0.008218842,"teacher_disagreement_score":0.0044876817,"about_ca_system_score_codex":0.00036785615,"about_ca_system_score_gemma":0.0000792115,"threshold_uncertainty_score":0.008923173},"labels":[],"label_agreement":null},{"id":"W4366181211","doi":"10.3847/1538-4357/ac78da","title":"Calibrating X-Ray Binary Luminosity Functions via Optical Reconnaissance. II. The High-mass XLF and Globular Cluster Population of X-Ray Binaries in the Low Star-forming Spiral M81","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Ontario College of Art and Design","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Astronomy; Galaxy; Spiral galaxy; Star cluster; Luminosity; Population; X-ray binary; Stellar mass; Surface brightness; Mass segregation; Star formation; Neutron star","score_opus":0.010035834088264823,"score_gpt":0.21388504406440303,"score_spread":0.2038492099761382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4366181211","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976914,0.00005103733,0.0015549229,0.000007919708,0.0000014555607,0.0000055320006,0.00011029183,0.00004213064,0.0005354456],"genre_scores_gemma":[0.9969459,0.000025756872,0.0024589112,0.0000075603475,0.000002444914,0.0000043258124,0.0003229023,0.000009205563,0.00022293701],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976116,0.000055955854,0.000013517782,0.0000923667,0.000042913765,0.00003410724],"domain_scores_gemma":[0.99919957,0.00015194327,0.00027709175,0.000184071,0.000114766204,0.00007272457],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006690526,0.0002776564,0.00017388751,0.001149714,0.00022297692,0.0006261139,0.00030401244,0.00024194617,0.0006815763],"category_scores_gemma":[0.0015395698,0.00019652245,0.0001609827,0.0005543851,0.0002489758,0.00039086014,0.00032525003,0.00014785425,0.0005378582],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000750239,0.000045519006,0.959737,0.000015928223,0.000035601985,0.000031636027,0.00011275596,0.0026926692,0.010608133,0.00014478595,0.0001343646,0.026366556],"study_design_scores_gemma":[0.0000051613097,0.00003439113,0.9834362,0.000004570369,0.000011607367,0.00006622948,0.00007704229,0.013459114,0.0025880479,0.00008246944,0.00023048997,0.0000046484247],"about_ca_topic_score_codex":0.0050630453,"about_ca_topic_score_gemma":0.009744746,"teacher_disagreement_score":0.0050630453,"about_ca_system_score_codex":0.0002986894,"about_ca_system_score_gemma":0.000116733296,"threshold_uncertainty_score":0.010067165},"labels":[],"label_agreement":null},{"id":"W4366401907","doi":"10.3847/1538-4357/acc6c2","title":"SPT-CL J2215−3537: A Massive Starburst at the Center of the Most Distant Relaxed Galaxy Cluster","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"National Science Foundation; NASA Headquarters; Argonne National Laboratory; U.S. Department of Energy; European Commission; Space Telescope Science Institute; University of Chicago; High Energy Physics; Smithsonian Astrophysical Observatory; Gordon and Betty Moore Foundation; Office of Science; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Physics; Galaxy; Center (category theory); Cluster (spacecraft); Astrophysics; Galaxy cluster; Astronomy; Brightest cluster galaxy","score_opus":0.00969442820016362,"score_gpt":0.2187390012033252,"score_spread":0.2090445730031616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4366401907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99908745,0.00004046398,0.000107786895,0.000032337397,0.0000059395807,0.000004260148,0.00022749303,0.000023887778,0.0004703166],"genre_scores_gemma":[0.9987446,0.000020648777,0.00013827263,0.000034042358,0.000010996844,0.0000028945717,0.00076001376,0.0000075843022,0.0002810212],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990726,0.0000045685247,0.0000044577732,0.000033687906,0.000022159284,0.00002789126],"domain_scores_gemma":[0.9996141,0.000008177099,0.00006773498,0.00002255071,0.000028330092,0.0002590305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011047078,0.00031188052,0.00034387765,0.00043053454,0.0006105565,0.0005011454,0.00045861097,0.00033629668,0.0022293504],"category_scores_gemma":[0.00025445755,0.00012945061,0.00021082377,0.00039879524,0.0003315159,0.00017767532,0.00066612597,0.00026560202,0.0005927534],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010264441,0.00016203446,0.8020508,0.00009480228,0.0002027369,0.014522023,0.00073801185,0.0012287588,0.16229029,0.0005142485,0.003340847,0.0138288895],"study_design_scores_gemma":[0.000047608606,0.00023920386,0.9877386,0.000014196783,0.00004210658,0.0037609697,0.00035402054,0.0015435468,0.003224893,0.00016792752,0.0028482766,0.000018634428],"about_ca_topic_score_codex":0.0071066935,"about_ca_topic_score_gemma":0.008892591,"teacher_disagreement_score":0.0071066935,"about_ca_system_score_codex":0.00040238377,"about_ca_system_score_gemma":0.00016629293,"threshold_uncertainty_score":0.014130652},"labels":[],"label_agreement":null},{"id":"W4366773278","doi":"10.3847/1538-4357/acbcd3","title":"UV–Optical Disk Reverberation Lags despite a Faint X-Ray Corona in the Active Galactic Nucleus Mrk 335","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"HORIZON EUROPE European Research Council; NSAF Joint Fund; Major Research Plan; Joint Fund of Astronomy; National Aeronautics and Space Administration; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Astrophysics; Active galactic nucleus; Balmer series; Flare; Reverberation mapping; Flux (metallurgy); Luminosity; Astronomy; Galaxy; Accretion (finance); Emission spectrum; Spectral line","score_opus":0.01646860515019588,"score_gpt":0.24989020072354798,"score_spread":0.2334215955733521,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4366773278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998949,0.000080009246,0.00008625861,0.000018992718,0.0000024922363,0.0000041639337,0.00035155602,0.00003724855,0.0004703196],"genre_scores_gemma":[0.9984762,0.000029660097,0.00026683885,0.000022142389,0.0000106474245,0.000004852704,0.0010028372,0.000016830621,0.0001701349],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998442,0.000012727213,0.000008931958,0.000053849442,0.000038127844,0.00004215512],"domain_scores_gemma":[0.9995672,0.000028413368,0.00018404673,0.00006957052,0.00006278966,0.00008792264],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024826205,0.00029836295,0.00040812502,0.0005568113,0.0004042957,0.00061004556,0.00027372976,0.000268648,0.0006781391],"category_scores_gemma":[0.00041724995,0.0001739182,0.00021173673,0.00035137896,0.00026514105,0.0002844211,0.00040056658,0.00034460047,0.0004749104],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010843027,0.00021900015,0.7744173,0.00009862153,0.00017969061,0.0013559763,0.0014884671,0.0007448353,0.19984089,0.00011954643,0.0011991725,0.019252203],"study_design_scores_gemma":[0.00000442385,0.00010177427,0.99729115,0.000003757439,0.000015853737,0.00018203227,0.00011949837,0.00018843295,0.0015288594,0.000009617116,0.0005491185,0.0000054879206],"about_ca_topic_score_codex":0.005013456,"about_ca_topic_score_gemma":0.010244893,"teacher_disagreement_score":0.005013456,"about_ca_system_score_codex":0.00029387083,"about_ca_system_score_gemma":0.00010704863,"threshold_uncertainty_score":0.009968579},"labels":[],"label_agreement":null},{"id":"W4367056813","doi":"10.3847/1538-4357/acc6c1","title":"CHIME/FRB Discovery of 25 Repeating Fast Radio Burst Sources","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":155,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of British Columbia, Okanagan Campus; Herzberg Institute of Astrophysics; Canadian Institute for Theoretical Astrophysics; Toronto Metropolitan University; University of Toronto; Canadian Institute for Advanced Research; Thompson Rivers University; University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Foundation for Innovation; National Science Foundation","keywords":"Physics; Sky; Astrophysics","score_opus":0.012263037166551,"score_gpt":0.3008861054146668,"score_spread":0.2886230682481158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367056813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933669,0.0004900473,0.0020856988,0.000117572,0.000017721473,0.000028891309,0.0010106293,0.00028055144,0.0026019695],"genre_scores_gemma":[0.99379116,0.00010800026,0.003358523,0.00006731242,0.000025357174,0.000015888012,0.0017349188,0.000044162083,0.0008546022],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997794,0.000012602015,0.000008645584,0.00008789829,0.00006199482,0.00004948105],"domain_scores_gemma":[0.99913293,0.000108241766,0.00029238017,0.00012771986,0.00009412624,0.0002445858],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038233548,0.00032624663,0.0003308254,0.0013565775,0.00046781922,0.0007412999,0.0003785372,0.00045797334,0.0021016141],"category_scores_gemma":[0.0008854788,0.0002861199,0.00028906082,0.0008381012,0.00030956927,0.00017907117,0.0006891507,0.0004212507,0.00071143947],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005129265,0.000069233385,0.82813025,0.000098511184,0.00026278818,0.0023566575,0.00078663725,0.00103011,0.12058001,0.0006228118,0.0022754886,0.043274604],"study_design_scores_gemma":[0.000019817311,0.000050855895,0.9870537,0.000016876125,0.000043925138,0.0009334203,0.00012481846,0.001006137,0.005456174,0.00017298764,0.0050940816,0.000027120039],"about_ca_topic_score_codex":0.0045518964,"about_ca_topic_score_gemma":0.006934132,"teacher_disagreement_score":0.0045518964,"about_ca_system_score_codex":0.0004535133,"about_ca_system_score_gemma":0.00014068038,"threshold_uncertainty_score":0.0090507865},"labels":[],"label_agreement":null},{"id":"W4367180699","doi":"10.3847/1538-4357/acc177","title":"Joint Modelling of Dust Scattering and Thermal Emission: The Spider Complex","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Centre National d’Etudes Spatiales; Bundesministerium für Verkehr, Innovation und Technologie; Centre National de la Recherche Scientifique; KU Leuven; Max-Planck-Institut für Astronomie; Cardiff University; National Aeronautics and Space Administration; California Institute of Technology; Government of Ontario; Imperial College London; UK Space Agency","keywords":"Cirrus; Physics; Brightness; Sky; Radiative transfer; Sky brightness; Cosmic dust; Scattering; Astrophysics; Extinction (optical mineralogy); Zodiacal light; Wavelength; Optical depth; Astronomy; Atmospheric sciences; Optics; Meteorology; Aerosol","score_opus":0.07355985979120538,"score_gpt":0.25932965276323366,"score_spread":0.18576979297202828,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367180699","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97310424,0.0000668494,0.025399711,0.00010648785,0.000005143931,0.000018232193,0.0001032286,0.00008778737,0.0011083657],"genre_scores_gemma":[0.99739945,0.000029812714,0.0021214138,0.000010490918,0.0000054479237,0.000006851433,0.00006689092,0.00003187667,0.00032773492],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998222,0.000050078157,0.000007911464,0.00005277059,0.000035399116,0.00003170679],"domain_scores_gemma":[0.99943763,0.00026781965,0.000096235664,0.000052306004,0.00005595023,0.000089974295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052182854,0.0005375269,0.00044607633,0.0005644013,0.00037916418,0.0011988607,0.0007596163,0.00055904285,0.0005742704],"category_scores_gemma":[0.0015581835,0.00035546016,0.0007501967,0.00041559164,0.0007031246,0.0006586855,0.0006261852,0.0004514068,0.000074836666],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011289385,0.0000672482,0.056125466,0.000022394197,0.000102137885,0.00031759424,0.00012135468,0.9259787,0.008523989,0.00490044,0.00025635402,0.0034714064],"study_design_scores_gemma":[0.000006115505,0.0000074374498,0.003601704,0.0000011162863,0.0000036438416,0.00002436749,0.000012703493,0.995363,0.00028167982,0.0006228753,0.00007026728,0.000005155005],"about_ca_topic_score_codex":0.016543128,"about_ca_topic_score_gemma":0.009446909,"teacher_disagreement_score":0.016543128,"about_ca_system_score_codex":0.00089690596,"about_ca_system_score_gemma":0.0004054584,"threshold_uncertainty_score":0.032893658},"labels":[],"label_agreement":null},{"id":"W4367180716","doi":"10.3847/1538-4357/acbfb7","title":"The SDSS-V Black Hole Mapper Reverberation Mapping Project: Unusual Broad-line Variability in a Luminous Quasar","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Quasar; Reverberation mapping; Emission spectrum; Radial velocity; Supermassive black hole; Spectral line; Line (geometry); Astronomy; Stars; Galaxy; Geometry","score_opus":0.025630267899286272,"score_gpt":0.26775385634528304,"score_spread":0.24212358844599677,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367180716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979487,0.000039864313,0.0007233415,0.000021864811,0.0000033601966,0.0000075055423,0.00094828435,0.00008123128,0.00022590726],"genre_scores_gemma":[0.994356,0.000025891004,0.0017335961,0.00001778102,0.000010103301,0.000009827078,0.0036065422,0.00003191522,0.00020825812],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996859,0.00006254274,0.000015626787,0.00007526611,0.00010016821,0.000060476],"domain_scores_gemma":[0.99923646,0.000095276526,0.0002610252,0.00013736315,0.00009653485,0.00017348588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010847826,0.0003214016,0.0002530275,0.0020039883,0.0003207114,0.0004723118,0.0003221176,0.00024511252,0.00042186558],"category_scores_gemma":[0.00090541155,0.00014886317,0.00024313269,0.0008302899,0.00022273086,0.00032982018,0.00072846166,0.0001932421,0.00018157765],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020012746,0.00020663344,0.9445802,0.000029231265,0.00015426661,0.00091650506,0.0007122147,0.0017756133,0.027508069,0.00019196466,0.0019809597,0.021744348],"study_design_scores_gemma":[0.000006839673,0.000037064598,0.9956514,0.0000028977795,0.000013526328,0.00021261108,0.00012729643,0.0018435488,0.0011127623,0.00005477589,0.000931532,0.0000057110287],"about_ca_topic_score_codex":0.003103697,"about_ca_topic_score_gemma":0.005432647,"teacher_disagreement_score":0.003103697,"about_ca_system_score_codex":0.00013039488,"about_ca_system_score_gemma":0.0001223965,"threshold_uncertainty_score":0.006171286},"labels":[],"label_agreement":null},{"id":"W4367842925","doi":"10.3847/1538-4357/acc39f","title":"Evidence of First Stars-enriched Gas in High-redshift Absorbers*","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"HORIZON EUROPE European Research Council; Horizon 2020 Framework Programme; Ministero dell’Istruzione, dell’Università e della Ricerca; European Commission; National Science Foundation","keywords":"Stars; Astrophysics; Physics; Supernova; Redshift; Population; Carbon fibers; Chemical composition; Metal; Astronomy; Materials science; Galaxy; Metallurgy","score_opus":0.0226938555527426,"score_gpt":0.24922374562938732,"score_spread":0.2265298900766447,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367842925","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99843806,0.00025971953,0.00038149313,0.000013823764,0.0000037282414,0.0000028349227,0.00009955009,0.0000467269,0.0007539861],"genre_scores_gemma":[0.99933606,0.000041894935,0.0002217798,0.000010285945,0.000006185328,0.0000015259529,0.00011176096,0.0000051918655,0.0002653504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998723,0.000007680654,0.0000044526723,0.000040066483,0.000027398193,0.000048065704],"domain_scores_gemma":[0.9995284,0.000056771038,0.00018621433,0.00003108157,0.00005825483,0.00013925582],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018825673,0.0002736914,0.0002356918,0.0015612072,0.00037323532,0.0006442152,0.00028743118,0.000404886,0.002370468],"category_scores_gemma":[0.00023986085,0.0001489444,0.00017180285,0.00057668344,0.00036239292,0.00024047085,0.00039073048,0.00027271616,0.0004252177],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029290662,0.00008639765,0.7056732,0.00009311811,0.00009988706,0.0005184166,0.00028124277,0.00017043715,0.28320295,0.00036893715,0.00024874185,0.008963683],"study_design_scores_gemma":[0.000004114494,0.00008315395,0.9841966,0.0000051235793,0.000023161814,0.00058715045,0.000090968264,0.00030477394,0.013831733,0.0000960493,0.0007728834,0.0000041775343],"about_ca_topic_score_codex":0.0010567956,"about_ca_topic_score_gemma":0.0012240281,"teacher_disagreement_score":0.002370468,"about_ca_system_score_codex":0.00023173016,"about_ca_system_score_gemma":0.000099706536,"threshold_uncertainty_score":0.00793004},"labels":[],"label_agreement":null},{"id":"W4367844022","doi":"10.3847/1538-4357/acbf46","title":"CLASSY. VI. The Density, Structure, and Size of Absorption-line Outflows in Starburst Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Space Telescope Science Institute; Carnegie Mellon University; Office of Science; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; George Mason University; European Space Agency; National Science Foundation; University of Washington; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Princeton University; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Galaxy; Astrophysics; Outflow; Star formation; RADIUS; Photoionization; Line (geometry); Absorption (acoustics); Optical depth; Electron density; Line-of-sight; Galaxy formation and evolution; Astronomy; Plasma; Ionization; Ion; Geometry; Meteorology","score_opus":0.009115476940002145,"score_gpt":0.22178240651052739,"score_spread":0.21266692957052524,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367844022","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99717724,0.00007701965,0.00009656476,0.000018301587,0.0000019840218,0.0000037710236,0.001430682,0.000013416518,0.0011810191],"genre_scores_gemma":[0.9972205,0.000054495158,0.00013787032,0.000012494609,0.0000073151145,0.000005349913,0.0019664,0.0000063632388,0.0005891396],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999286,0.000004680279,0.0000041356843,0.000029398598,0.000014153033,0.000019011508],"domain_scores_gemma":[0.9991731,0.00007311067,0.00042443894,0.000051687228,0.00009078938,0.00018686922],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015107823,0.00012230258,0.00013646144,0.0009571699,0.0003272584,0.0005178104,0.00018668339,0.0001618926,0.003932838],"category_scores_gemma":[0.0005411008,0.0000720232,0.00010482449,0.0005405745,0.00019238464,0.00031844797,0.00038973836,0.00013089318,0.0006430378],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000020731166,0.000009864593,0.9953733,0.0000051796096,0.000005884567,0.000010685451,0.00007253029,0.000054072872,0.0012578827,0.00003861349,0.00022646216,0.0029248362],"study_design_scores_gemma":[6.358581e-7,0.000003675822,0.99968076,7.770247e-7,6.915853e-7,0.0000099055815,0.000034374312,0.000065212764,0.00007615939,0.000008517697,0.00011907614,3.4247842e-7],"about_ca_topic_score_codex":0.014998938,"about_ca_topic_score_gemma":0.019360514,"teacher_disagreement_score":0.014998938,"about_ca_system_score_codex":0.00037726638,"about_ca_system_score_gemma":0.00013766252,"threshold_uncertainty_score":0.029823303},"labels":[],"label_agreement":null},{"id":"W4367844043","doi":"10.3847/1538-4357/acc100","title":"Carnegie Supernova Project. II. Near-infrared Spectral Diversity and Template of Type Ia Supernovae","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Rio Tinto (Canada); Espace pour la vie","funders":"Division of Astronomical Sciences; European Social Fund; Fundação para a Ciência e a Tecnologia; Ministerio de Ciencia e Innovación; Space Telescope Science Institute; Astrophysics Science Division; Villum Fonden","keywords":"Physics; Supernova; Light curve; Astrophysics; Spectral line; Spectral shape analysis; Principal component analysis; Spectrograph; Astronomy; Statistics","score_opus":0.024578705496300274,"score_gpt":0.25560252135157796,"score_spread":0.23102381585527768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4367844043","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.82589597,0.0006443226,0.02084988,0.0002844821,0.00006678785,0.00044942016,0.14086658,0.0019479592,0.008994645],"genre_scores_gemma":[0.7572203,0.00023640497,0.039482605,0.000093316514,0.000026094063,0.00036196303,0.19958416,0.0005642952,0.0024307838],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994017,0.00007043064,0.0000357219,0.00022405833,0.0001901785,0.00007792318],"domain_scores_gemma":[0.99773264,0.00017824098,0.0005690378,0.00079005264,0.0004059635,0.000324066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018758184,0.0006442312,0.00042588884,0.002449544,0.0006052526,0.0007887479,0.0008113845,0.00039468036,0.002011388],"category_scores_gemma":[0.002871333,0.00044837114,0.0007024676,0.002301611,0.00025998757,0.00043444432,0.0007945722,0.00043611004,0.0010096899],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00087135565,0.00025408086,0.8609126,0.00021431125,0.0006173129,0.00026918773,0.0002254424,0.013077459,0.024970405,0.003497631,0.01852853,0.07656169],"study_design_scores_gemma":[0.0000414055,0.00012500791,0.96498656,0.000022253946,0.000071804636,0.00038407484,0.000058912647,0.011181384,0.008038533,0.0010611987,0.013989973,0.000038780378],"about_ca_topic_score_codex":0.02052275,"about_ca_topic_score_gemma":0.03520721,"teacher_disagreement_score":0.02052275,"about_ca_system_score_codex":0.0005823714,"about_ca_system_score_gemma":0.00082995015,"threshold_uncertainty_score":0.04080659},"labels":[],"label_agreement":null},{"id":"W4368405228","doi":"10.3847/1538-4357/ac940c","title":"Comparing Be Star Inclination Angles Determined from Hα Fitting and Gravitational Darkening","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Stars; Radiative transfer; Line-of-sight; Light curve; Line (geometry); Rotation (mathematics); Be star; Optics; Geometry","score_opus":0.026625583267605273,"score_gpt":0.2571499759876869,"score_spread":0.23052439272008163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4368405228","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979109,0.00005414583,0.00074984087,0.000006032819,0.0000021854798,0.000004046421,0.00031995206,0.00002605195,0.0009268429],"genre_scores_gemma":[0.997355,0.000040140207,0.0007517789,0.0000065261916,0.000002644947,0.0000039976376,0.0016172109,0.000014224596,0.0002085584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99954814,0.00008373603,0.00005366721,0.00013228755,0.00012446908,0.000057724516],"domain_scores_gemma":[0.9981164,0.00031582481,0.00058807,0.00027041454,0.00050521345,0.00020413676],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008072255,0.00029591736,0.00038537086,0.0016022255,0.0002507862,0.00064148393,0.00016906833,0.0002565386,0.0007424318],"category_scores_gemma":[0.00298841,0.00015900073,0.00020545248,0.0010828205,0.00016261278,0.00029296614,0.00057664444,0.00018368436,0.0010000465],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001811874,0.00001974004,0.9840868,0.000015392163,0.000060781003,0.000028637789,0.00012453458,0.00074482977,0.007295637,0.00006105742,0.00014999977,0.0072313272],"study_design_scores_gemma":[0.000003758567,0.000042021977,0.99478513,0.0000032370974,0.000012527768,0.00008432081,0.00009673174,0.0017034458,0.0028014972,0.000054883825,0.00040855122,0.0000038981143],"about_ca_topic_score_codex":0.0012564487,"about_ca_topic_score_gemma":0.002220315,"teacher_disagreement_score":0.0016022255,"about_ca_system_score_codex":0.00015771513,"about_ca_system_score_gemma":0.000071022114,"threshold_uncertainty_score":0.0042690635},"labels":[],"label_agreement":null},{"id":"W4375847853","doi":"10.3847/1538-4357/acc38d","title":"Redshift Evolution of the Feedback–Cooling Equilibrium in the Core of 48 SPT Galaxy Clusters: A Joint Chandra–SPT–ATCA Analysis","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Argonne National Laboratory; U.S. Department of Energy; European Commission; University of Chicago; High Energy Physics; Smithsonian Astrophysical Observatory; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Smithsonian Institution; National Science Foundation","keywords":"Physics; Redshift; Astrophysics; Galaxy; South Pole Telescope; Cluster (spacecraft); Active galactic nucleus; Luminosity; Galaxy cluster; RADIUS","score_opus":0.015932952447189643,"score_gpt":0.23079381054122838,"score_spread":0.21486085809403874,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4375847853","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99931765,0.000023385046,0.00024406848,0.000007410961,6.652523e-7,0.0000029939392,0.00023128356,0.000030134224,0.00014241332],"genre_scores_gemma":[0.9991273,0.000008550239,0.00023190603,0.0000027596543,0.0000026965347,0.000002678961,0.0005480274,0.000009145918,0.00006688416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983466,0.000022664575,0.000008728394,0.00004811893,0.000042419433,0.00004337724],"domain_scores_gemma":[0.9985858,0.0003638165,0.00038472645,0.00022537171,0.00018130883,0.00025900698],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000523351,0.00025168445,0.0003825349,0.002093943,0.00045310668,0.0006024138,0.00041716083,0.00020465204,0.0013158495],"category_scores_gemma":[0.001557599,0.00023503497,0.0007014768,0.0010112119,0.00037489156,0.0002702737,0.0007408991,0.00026638413,0.0002303828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035731733,0.00004521946,0.968635,0.000020657755,0.00016812448,0.00016111191,0.00023311764,0.011627132,0.011111735,0.0004726657,0.00045916348,0.0067087538],"study_design_scores_gemma":[0.0000066377993,0.00002467872,0.9811329,0.00000179333,0.000027324826,0.000049171973,0.000035237103,0.01771822,0.0007427343,0.00007117819,0.00018243611,0.000007618044],"about_ca_topic_score_codex":0.01683361,"about_ca_topic_score_gemma":0.008565689,"teacher_disagreement_score":0.01683361,"about_ca_system_score_codex":0.00055349566,"about_ca_system_score_gemma":0.0002011936,"threshold_uncertainty_score":0.033471227},"labels":[],"label_agreement":null},{"id":"W4376106026","doi":"10.3847/1538-4357/acc184","title":"The Fast X-Ray Transient XRT 210423 and Its Host Galaxy","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Leibniz-Gemeinschaft; Science and Technology Facilities Council; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; Yale University; Vanderbilt University; New Mexico State University; University of Portsmouth; University of Washington; University of Notre Dame; Ohio State University; Ministerio de Ciencia e Innovación; York University","keywords":"Physics; Transient (computer programming); Galaxy; Astrophysics; Host (biology); X-ray transient; Astronomy; Neutron star","score_opus":0.011152999899956282,"score_gpt":0.22833274474980114,"score_spread":0.21717974484984487,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376106026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99648017,0.0001131486,0.00014550198,0.00004634827,0.000007986308,0.000008090596,0.0002326335,0.000030828378,0.0029354335],"genre_scores_gemma":[0.9983187,0.00003126059,0.0002599727,0.000031414264,0.000011200299,0.000003674134,0.0007093519,0.000006835938,0.0006275945],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992967,0.000004248567,0.0000037851162,0.000021105925,0.000016860844,0.000024370785],"domain_scores_gemma":[0.9998134,0.000012084554,0.0000602278,0.000018640629,0.000016142247,0.00007968066],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000101106896,0.0002702227,0.00021732923,0.00071873015,0.0006302777,0.00064929837,0.00020986688,0.00041614924,0.0020705054],"category_scores_gemma":[0.0001865382,0.00015750984,0.00019287191,0.0005766205,0.0002278753,0.00020508235,0.00044309994,0.00024051967,0.0006859557],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008362569,0.00030965477,0.8893632,0.00008126336,0.00005575798,0.006130598,0.00069245143,0.0007757603,0.07983492,0.0016085956,0.0023115703,0.017999995],"study_design_scores_gemma":[0.00002303713,0.00018091268,0.98898005,0.000012605308,0.00001675998,0.00285162,0.00028946679,0.000983578,0.002370778,0.00019294344,0.0040883464,0.000009817079],"about_ca_topic_score_codex":0.003337616,"about_ca_topic_score_gemma":0.0038056455,"teacher_disagreement_score":0.003337616,"about_ca_system_score_codex":0.00032272158,"about_ca_system_score_gemma":0.00017411166,"threshold_uncertainty_score":0.006926596},"labels":[],"label_agreement":null},{"id":"W4376106114","doi":"10.3847/1538-4357/acbf1e","title":"JWST Observations of the Enigmatic Y-Dwarf WISE 1828+2650. I. Limits to a Binary Companion","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; Science Mission Directorate; Goddard Space Flight Center; Canadian Space Agency; Jet Propulsion Laboratory; Space Telescope Science Institute; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation","keywords":"Physics; Brown dwarf; James Webb Space Telescope; Photometry (optics); Planet; Astronomy; Astrophysics; Binary number; Exoplanet; Spectroscopy; Circumbinary planet; Telescope; Stars","score_opus":0.03405423533597246,"score_gpt":0.24988200704025984,"score_spread":0.21582777170428738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376106114","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99370414,0.00023889972,0.00032483946,0.00004904969,0.000009577099,0.0000066797616,0.0004806471,0.000052449934,0.005133615],"genre_scores_gemma":[0.9976858,0.000053177326,0.00052345777,0.000028886381,0.000011864243,0.0000051292986,0.0007242697,0.00001030689,0.00095710706],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999213,0.0000041842445,0.000005027912,0.00002423777,0.000028369217,0.000016847474],"domain_scores_gemma":[0.9996575,0.000033029675,0.000105243045,0.000032094806,0.000056213514,0.00011588776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014749067,0.00015431967,0.00019149063,0.0005366972,0.00042989946,0.00036969624,0.00021983199,0.00023315565,0.001734184],"category_scores_gemma":[0.00034333536,0.00017278577,0.000098925884,0.00036830758,0.00021830491,0.00027274166,0.00046722224,0.00021641134,0.00069736125],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054390065,0.00013450498,0.73147386,0.00015364146,0.000058992326,0.0015206329,0.00055146625,0.00055791036,0.23703673,0.0008745603,0.003674309,0.023419509],"study_design_scores_gemma":[0.000020367459,0.00011316696,0.98856634,0.00001259135,0.000024049574,0.0005171754,0.00021948264,0.0005341883,0.0049651377,0.00014482572,0.0048755966,0.0000071760114],"about_ca_topic_score_codex":0.0034726819,"about_ca_topic_score_gemma":0.010109776,"teacher_disagreement_score":0.0034726819,"about_ca_system_score_codex":0.00024851592,"about_ca_system_score_gemma":0.0001206593,"threshold_uncertainty_score":0.0069049597},"labels":[],"label_agreement":null},{"id":"W4376122196","doi":"10.3847/1538-4357/acc06d","title":"Self-consistent Spin, Tidal, and Dynamical Equations of Motion in the REBOUNDx Framework","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; The Scarborough Hospital; University of Toronto","funders":"","keywords":"Physics; Equations of motion; Classical mechanics; Test particle; Benchmark (surveying); Motion (physics); Dynamical systems theory; Constant (computer programming); Integrator; Tidal acceleration; Spin (aerodynamics); Lag; Statistical physics; Astrophysics; Quantum mechanics; Geodesy","score_opus":0.015056619889085531,"score_gpt":0.25310996670729974,"score_spread":0.23805334681821422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376122196","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.179861,0.001189881,0.75259125,0.0016617061,0.0005330523,0.00022270442,0.0021994847,0.0013520898,0.060388867],"genre_scores_gemma":[0.7211973,0.0007990934,0.23306352,0.00085951405,0.00029820937,0.0005195547,0.0018285379,0.0014783922,0.03995593],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997212,0.0000897861,0.000012476251,0.000029118299,0.000111946785,0.000035401215],"domain_scores_gemma":[0.999469,0.00014100254,0.00007301413,0.0000920774,0.00015007654,0.00007483648],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096947985,0.0005635786,0.0010968973,0.0006013849,0.00068058,0.001344338,0.0020199884,0.0010196476,0.0057271337],"category_scores_gemma":[0.0016212711,0.0005524397,0.000725688,0.0004936149,0.0012070311,0.0014234084,0.0020507348,0.0012522587,0.00094607053],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006773301,0.00005990057,0.0011587664,0.00007318141,0.000031479194,0.00019031478,0.00010757648,0.6800954,0.0014838413,0.30515835,0.0042100367,0.0073634777],"study_design_scores_gemma":[0.000031492942,0.0000093967,0.00017101945,0.000009457294,0.0000032257321,0.000017455995,0.000013772715,0.97701716,0.00018475886,0.020335134,0.0021973418,0.000009702382],"about_ca_topic_score_codex":0.017055523,"about_ca_topic_score_gemma":0.012417825,"teacher_disagreement_score":0.017055523,"about_ca_system_score_codex":0.0011967244,"about_ca_system_score_gemma":0.001468491,"threshold_uncertainty_score":0.03391248},"labels":[],"label_agreement":null},{"id":"W4376123236","doi":"10.3847/1538-4357/acaf51","title":"The Rest-frame Submillimeter Spectrum of High-redshift, Dusty, Star-forming Galaxies from the SPT-SZ Survey","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Comisión Nacional de Investigación Científica y Tecnológica; Max-Planck-Gesellschaft; Consejo Nacional de Innovación, Ciencia y Tecnología; Fondo Nacional de Desarrollo Científico y Tecnológico; Danmarks Grundforskningsfond; National Astronomical Observatory of Japan; National Research Foundation; Alfred P. Sloan Foundation; Agencia Nacional de Investigación y Desarrollo; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Rest frame; Redshift; Astrophysics; Galaxy; Rest (music); Astronomy; Star (game theory); Star formation; Redshift survey; Luminous infrared galaxy","score_opus":0.0137070899607028,"score_gpt":0.22109525445480394,"score_spread":0.20738816449410113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376123236","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9887318,0.00007065593,0.00033411375,0.000031107844,0.000004519321,0.000011772857,0.009592365,0.00009267154,0.0011310487],"genre_scores_gemma":[0.96010596,0.00014884399,0.0009921154,0.000044593107,0.000031234227,0.000018196555,0.03770031,0.000042631422,0.0009161183],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999811,0.000012534333,0.000011880991,0.000048789196,0.00007268176,0.000043110795],"domain_scores_gemma":[0.99933225,0.00003888422,0.00017304099,0.00008522198,0.00016210585,0.00020844024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027248278,0.00032542157,0.00034578764,0.0018878253,0.00027054726,0.0005121634,0.00029968092,0.00013980035,0.0026844726],"category_scores_gemma":[0.00053164444,0.00015990049,0.00029056252,0.0017551708,0.0001592037,0.00028035475,0.0006193618,0.00023303962,0.0013028038],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007423015,0.000030044393,0.974912,0.000032322198,0.000076563454,0.00014676867,0.00029405332,0.00026159603,0.0076549156,0.00007315901,0.0035835463,0.01286077],"study_design_scores_gemma":[0.0000017749333,0.000011853597,0.9989146,0.0000011292938,0.000006570972,0.00009112992,0.00003904455,0.00012301512,0.00020753883,0.000008935542,0.0005929861,0.0000014096828],"about_ca_topic_score_codex":0.00895788,"about_ca_topic_score_gemma":0.011917408,"teacher_disagreement_score":0.00895788,"about_ca_system_score_codex":0.00025663892,"about_ca_system_score_gemma":0.00016656112,"threshold_uncertainty_score":0.017811477},"labels":[],"label_agreement":null},{"id":"W4376128714","doi":"10.3847/1538-4357/ac4ccb","title":"The Magnificent Five Images of Supernova Refsdal: Time Delay and Magnification Measurements","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Agencia Estatal de Investigación; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España; European Commission; UK Research and Innovation; Space Telescope Science Institute; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; European Research Council; Nuclear Safety and Security Commission; Ministerio de Ciencia, Innovación y Universidades; Gordon and Betty Moore Foundation; Jet Propulsion Laboratory; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Villum Fonden; Ministerio de Economía y Competitividad; NASA Headquarters; National Science Foundation","keywords":"Physics; Magnification; Gravitational microlensing; Galaxy; Photometry (optics); Astrophysics; Supernova; Brightness; Telescope; Astronomy; Stars; Optics","score_opus":0.017730738075344993,"score_gpt":0.24406881818534093,"score_spread":0.22633808010999593,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376128714","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9358606,0.0004183046,0.036155954,0.0001764562,0.00011896501,0.000119754186,0.0077519505,0.004302099,0.015095937],"genre_scores_gemma":[0.9377816,0.000089937326,0.052232213,0.00008002068,0.000049656555,0.000035901947,0.0074455077,0.00045230731,0.0018329917],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99969816,0.000016592941,0.000018929104,0.00008528782,0.0001252818,0.00005584475],"domain_scores_gemma":[0.9988475,0.00016706245,0.00019964004,0.00018779628,0.00034533348,0.0002526275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057826313,0.00030115593,0.0001970696,0.0024675673,0.00022369197,0.00062027626,0.00039374968,0.00030240172,0.0047919163],"category_scores_gemma":[0.0014786763,0.0002780482,0.00036648056,0.00063349784,0.00021454197,0.0004473988,0.0006633483,0.0004118167,0.0008998322],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019165401,0.00025028607,0.35557854,0.00041438383,0.00037710633,0.0007829127,0.0007976249,0.0055288547,0.41915458,0.004631585,0.010510578,0.20005694],"study_design_scores_gemma":[0.000063140986,0.00023784136,0.75264996,0.000046456167,0.00010523512,0.0011519353,0.0001872205,0.031712577,0.19439644,0.0014250926,0.017911565,0.000112493486],"about_ca_topic_score_codex":0.0020911132,"about_ca_topic_score_gemma":0.005377172,"teacher_disagreement_score":0.0047919163,"about_ca_system_score_codex":0.0006540265,"about_ca_system_score_gemma":0.00018795382,"threshold_uncertainty_score":0.01603055},"labels":[],"label_agreement":null},{"id":"W4376163549","doi":"10.3847/1538-4357/accc89","title":"Coronal Heating as Determined by the Solar Flare Frequency Distribution Obtained by Aggregating Case Studies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"McGill University; Division of Materials Research; National Aeronautics and Space Administration; National Centers for Environmental Information; National Oceanic and Atmospheric Administration; National Science Foundation","keywords":"Physics; Flare; Nanoflares; Astrophysics; Solar flare; Coronal loop; Magnetic reconnection; Solar physics; Coronal mass ejection; Corona (planetary geology); Astronomy; Plasma; Solar wind; Nuclear physics","score_opus":0.011617904695534127,"score_gpt":0.26923280181329257,"score_spread":0.2576148971177584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376163549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971011,0.000039219303,0.00191888,0.000011821341,0.0000019405848,0.000022172202,0.00020772767,0.000027390115,0.0006697999],"genre_scores_gemma":[0.9969137,0.000025637893,0.0023718583,0.0000042902584,0.000004495925,0.000013843142,0.00053638895,0.0000058641717,0.00012380419],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986268,0.000342252,0.00012699801,0.00032055436,0.00040358826,0.00017984281],"domain_scores_gemma":[0.98337287,0.010074289,0.0017142426,0.0019782295,0.0024498692,0.0004105555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023266121,0.0003162988,0.00035553062,0.0038490982,0.00054515374,0.0009227264,0.00045167108,0.00040686622,0.0007439176],"category_scores_gemma":[0.010586049,0.0001607842,0.00055673084,0.0023075214,0.0005454245,0.00058286556,0.00067754736,0.00030457033,0.00015338445],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022968331,0.00027380418,0.9198096,0.00007528645,0.00035594104,0.0012128054,0.000988868,0.02747111,0.009143254,0.0010809958,0.00075573084,0.038603067],"study_design_scores_gemma":[0.0000122581305,0.0004109209,0.83388144,0.00002252694,0.00025354678,0.001571206,0.0024054702,0.1464566,0.010978838,0.0019742674,0.001975439,0.000057496363],"about_ca_topic_score_codex":0.002839049,"about_ca_topic_score_gemma":0.0030745235,"teacher_disagreement_score":0.0038490982,"about_ca_system_score_codex":0.0004518041,"about_ca_system_score_gemma":0.00015117724,"threshold_uncertainty_score":0.012304425},"labels":[],"label_agreement":null},{"id":"W4376274741","doi":"10.3847/1538-4357/acc325","title":"Multiple Rings and Asymmetric Structures in the Disk of SR 21","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Jet Propulsion Laboratory","keywords":"Physics; Astrophysics; Millimeter; Planet; Submillimeter Array; Protoplanetary disk; T Tauri star; Wavelength; Star formation; Astronomy; Stars; Optics","score_opus":0.011159060762480804,"score_gpt":0.24340584774415353,"score_spread":0.23224678698167273,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376274741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99954057,0.00004532051,0.000096422795,0.00000811388,0.0000012536768,0.0000010519892,0.0000473304,0.000010603963,0.00024942806],"genre_scores_gemma":[0.99944955,0.000019740626,0.00030736098,0.0000033740744,0.00000386511,0.0000010891464,0.00012725899,0.0000032712633,0.00008448503],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992967,0.0000055253927,0.0000052525434,0.00002432982,0.000016985503,0.000018253275],"domain_scores_gemma":[0.99976915,0.000023824172,0.00009178833,0.000030243906,0.00003554846,0.00004948724],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000071972805,0.00014675417,0.00018103016,0.00073427614,0.00028256347,0.0003900703,0.00019584791,0.00020937981,0.0005653506],"category_scores_gemma":[0.00019822048,0.00011793439,0.00019037194,0.00034169955,0.00017203679,0.00023655653,0.00022358833,0.00013816144,0.00022901663],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045403605,0.00010531886,0.36679202,0.00009787716,0.00010217575,0.003175875,0.0009640913,0.0029803033,0.604351,0.0004514702,0.0005868224,0.01993906],"study_design_scores_gemma":[0.000016511905,0.00010354909,0.9790491,0.0000051529382,0.000026378326,0.001336473,0.00039769622,0.0069108447,0.010843375,0.0001424418,0.0011553615,0.000013034641],"about_ca_topic_score_codex":0.0010040771,"about_ca_topic_score_gemma":0.0010264331,"teacher_disagreement_score":0.0010040771,"about_ca_system_score_codex":0.0001393711,"about_ca_system_score_gemma":0.00006661271,"threshold_uncertainty_score":0.0019965172},"labels":[],"label_agreement":null},{"id":"W4376274856","doi":"10.3847/1538-4357/acc1e6","title":"CLEAR: High-ionization [Ne v] λ3426 Emission-line Galaxies at 1.4 &lt; z &lt; 2.3","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Doubly ionized oxygen; Emission spectrum; Active galactic nucleus; QSOS; Reionization; Lambda; Photoionization; Ionization; Quasar; Redshift; Astronomy; Spectral line","score_opus":0.009063692439440751,"score_gpt":0.2198559645188074,"score_spread":0.21079227207936665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376274856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981229,0.000036845933,0.000115079936,0.000019743153,0.0000013036931,0.00000512777,0.0011420005,0.000030348785,0.0005266747],"genre_scores_gemma":[0.9965758,0.000028237033,0.00020091102,0.00001725896,0.0000045048973,0.0000046542455,0.0024433297,0.00001003721,0.0007151887],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998448,0.0000074872364,0.00000426263,0.000037402602,0.00003543244,0.00007057141],"domain_scores_gemma":[0.99946815,0.000017475513,0.00023390944,0.00003122685,0.00004324926,0.0002060428],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001611793,0.00025942104,0.00019573068,0.0015159039,0.0003176702,0.00065895985,0.000271361,0.0001580519,0.0018389742],"category_scores_gemma":[0.00022754114,0.00015013215,0.00024448652,0.0006843865,0.0002169969,0.00023563675,0.00041350865,0.00022373997,0.0005165371],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000107754124,0.000055809734,0.9861801,0.000008467317,0.000038449543,0.00016699873,0.00013994137,0.00022959807,0.008769585,0.00013782158,0.000815144,0.003350285],"study_design_scores_gemma":[0.0000023825849,0.000010237674,0.99916315,0.0000010594244,0.000005072276,0.00004408478,0.000045845638,0.00010270694,0.00033836142,0.000008599882,0.0002768244,0.0000016956814],"about_ca_topic_score_codex":0.014504302,"about_ca_topic_score_gemma":0.027538802,"teacher_disagreement_score":0.014504302,"about_ca_system_score_codex":0.0002762743,"about_ca_system_score_gemma":0.00017625155,"threshold_uncertainty_score":0.028839767},"labels":[],"label_agreement":null},{"id":"W4376610663","doi":"10.3847/1538-4357/acc06e","title":"The Diffuse Ionized Gas Halo of the Large Magellanic Cloud","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada; University of British Columbia, Okanagan Campus; University of British Columbia","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Ionization; Halo; Galaxy; Galactic halo; Large Magellanic Cloud; Line-of-sight; Emission spectrum; Line (geometry); Spectral line; Hydrogen line; Plasma; Astronomy; Ion","score_opus":0.008894718905192,"score_gpt":0.23296245673639038,"score_spread":0.22406773783119838,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376610663","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9886973,0.0006700794,0.0005452982,0.000087137705,0.0000054278394,0.000007740796,0.0009533285,0.000109816945,0.00892388],"genre_scores_gemma":[0.9981495,0.00018408304,0.00025156463,0.00002460027,0.0000068430822,0.0000020409623,0.0004644961,0.0000143090065,0.0009025073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99997187,0.0000024741864,8.664058e-7,0.0000073578153,0.0000063506654,0.000011157442],"domain_scores_gemma":[0.999946,0.0000052935075,0.0000133945605,0.000005867274,0.000005231622,0.000024220068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000036989106,0.00013492508,0.000061578685,0.00036312419,0.00019147128,0.00042909742,0.00018124365,0.00006947034,0.002915825],"category_scores_gemma":[0.00013905542,0.000067920606,0.00007064129,0.00050659874,0.00018696894,0.00020440007,0.00034857783,0.00007929471,0.00032641774],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004950815,0.00006950109,0.6972683,0.00021426512,0.00014027335,0.002346783,0.0008727331,0.004761432,0.21347353,0.0066249194,0.007216991,0.06651616],"study_design_scores_gemma":[0.000026764134,0.00007198789,0.9621092,0.00005823905,0.000043722946,0.0004695324,0.00046828226,0.0017701844,0.011334929,0.0010881084,0.022541666,0.000017358943],"about_ca_topic_score_codex":0.019871917,"about_ca_topic_score_gemma":0.023369944,"teacher_disagreement_score":0.019871917,"about_ca_system_score_codex":0.00048228464,"about_ca_system_score_gemma":0.0001550783,"threshold_uncertainty_score":0.039512515},"labels":[],"label_agreement":null},{"id":"W4376873482","doi":"10.3847/1538-4357/acc584","title":"Detection of Interstellar E-1-cyano-1,3-butadiene in GOTHAM Observations of TMC-1","year":2023,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Astrophysics; Astrochemistry; Polycyclic aromatic hydrocarbon; Molecule; Abundance (ecology); Interstellar medium; Galaxy","score_opus":0.02419674134701092,"score_gpt":0.2466987922618374,"score_spread":0.2225020509148265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376873482","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9952428,0.00006653382,0.00032688503,0.00006315941,0.0000058783207,0.000012601259,0.00052325474,0.0000819128,0.0036768974],"genre_scores_gemma":[0.9976913,0.000032440737,0.0006262059,0.00008341858,0.000003757731,0.000010088332,0.0005526139,0.000019131605,0.0009809979],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999843,0.000005417071,0.0000025581478,0.00004035298,0.00005189669,0.000056858054],"domain_scores_gemma":[0.99981135,0.000014605515,0.000034490622,0.0000329396,0.000040296443,0.00006638553],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000110398,0.00022330393,0.00016920171,0.00066181284,0.0007754058,0.00036613413,0.00044716158,0.0004822743,0.0016512971],"category_scores_gemma":[0.00021337079,0.00019494283,0.00016274402,0.00050057605,0.00029965234,0.00013520493,0.0006206547,0.0005586535,0.00029070635],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041848677,0.00013702475,0.19771588,0.00008882845,0.00008828971,0.0017562131,0.0013398046,0.00091390917,0.78079873,0.0005686583,0.0024807742,0.013693323],"study_design_scores_gemma":[0.000025350168,0.000135716,0.9331933,0.000012644894,0.000043204578,0.00045612702,0.00037846732,0.0012873503,0.058606904,0.0001207341,0.005720267,0.000020017598],"about_ca_topic_score_codex":0.021221744,"about_ca_topic_score_gemma":0.06556351,"teacher_disagreement_score":0.021221744,"about_ca_system_score_codex":0.0008356487,"about_ca_system_score_gemma":0.00028692684,"threshold_uncertainty_score":0.042196453},"labels":[],"label_agreement":null},{"id":"W4376954856","doi":"10.3847/1538-4357/acc1e5","title":"FAUST. VII. Detection of a Hot Corino in the Prototypical Warm Carbon-chain Chemistry Source IRAS 15398–3359","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"RIKEN; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Protostar; Physics; Astrochemistry; Astrophysics; Excitation; Submillimeter Array; Carbon chain; Millimeter; Excitation temperature; Crossed molecular beam; Analytical Chemistry (journal); Atomic carbon; Molecule; Emission spectrum; Star formation; Hydrogen; Chemistry; Spectral line; Astronomy; Stars; Interstellar medium","score_opus":0.01085457487524843,"score_gpt":0.2345339435720671,"score_spread":0.22367936869681868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376954856","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8947498,0.0004261378,0.0051100557,0.0008666506,0.00007695803,0.00013270057,0.04325018,0.021955105,0.033432268],"genre_scores_gemma":[0.9454941,0.00008388795,0.01217472,0.00019981738,0.000032271102,0.000056545312,0.033074915,0.0014407845,0.007442898],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989724,0.000012654543,0.0000037278764,0.000027848002,0.00003181324,0.000026756219],"domain_scores_gemma":[0.99961394,0.00005704923,0.00009936098,0.0000912326,0.000051491443,0.00008694408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040221348,0.0003856404,0.0001602488,0.00089008553,0.0005685835,0.00034480766,0.00038761392,0.00022778861,0.005955305],"category_scores_gemma":[0.0005322501,0.00018033244,0.00021327213,0.00060673343,0.0001931301,0.00018729617,0.00027597786,0.00022865618,0.0027920352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023492079,0.0003860268,0.4551031,0.00034955624,0.00025330455,0.0022738979,0.0015672509,0.01060705,0.21067405,0.0027575083,0.14839266,0.16528638],"study_design_scores_gemma":[0.00020146063,0.00020033178,0.8448965,0.000040114453,0.000057785914,0.00067616947,0.00016683667,0.018343052,0.04287994,0.0007575025,0.091719896,0.00006047884],"about_ca_topic_score_codex":0.025026707,"about_ca_topic_score_gemma":0.039117336,"teacher_disagreement_score":0.025026707,"about_ca_system_score_codex":0.00069273845,"about_ca_system_score_gemma":0.00025716575,"threshold_uncertainty_score":0.04976207},"labels":[],"label_agreement":null},{"id":"W4376983037","doi":"10.3847/1538-4357/acc45a","title":"AGN STORM 2. II. Ultraviolet Observations of Mrk 817 with the Cosmic Origins Spectrograph on the Hubble Space Telescope*","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Herzberg Institute of Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; University of California, Irvine; Israel Science Foundation; Nuclear Safety and Security Commission; Space Telescope Science Institute; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Consejo Nacional de Ciencia y Tecnología; Wayne State University; National Science Foundation","keywords":"Space Telescope Imaging Spectrograph; Physics; Ultraviolet; Astrophysics; Hubble space telescope; Stars; Optics","score_opus":0.015559072780578626,"score_gpt":0.2233277312996705,"score_spread":0.20776865851909188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4376983037","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954888,0.000047051006,0.00051337207,0.000026275535,0.000007604075,0.0000112333155,0.0012028549,0.00016928892,0.0025334654],"genre_scores_gemma":[0.9936999,0.000031043288,0.0015193922,0.000028261271,0.00001865789,0.000009763882,0.0034154279,0.000052096908,0.0012253679],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998772,0.000011163516,0.000005277488,0.000029264163,0.000050673523,0.000026457239],"domain_scores_gemma":[0.9997708,0.000019516465,0.000066236134,0.000038126283,0.000037611295,0.00006757397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022800546,0.00021727495,0.00015656976,0.00063535443,0.00022417237,0.00026017008,0.00022390834,0.0001606207,0.0014369929],"category_scores_gemma":[0.00024711527,0.00013045693,0.00020881956,0.0002883512,0.0000899952,0.00015681046,0.0002741058,0.00025552895,0.0005755704],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013724439,0.0002533051,0.7248952,0.0000935106,0.00021294637,0.0011486878,0.000691987,0.002443485,0.21060634,0.00062566996,0.006411099,0.05124536],"study_design_scores_gemma":[0.000039511266,0.00014611261,0.9808257,0.000005307559,0.000033999957,0.00023424873,0.000058089157,0.0019389481,0.0136541445,0.00007923493,0.0029729935,0.000011620181],"about_ca_topic_score_codex":0.0026342585,"about_ca_topic_score_gemma":0.0077514797,"teacher_disagreement_score":0.0026342585,"about_ca_system_score_codex":0.00024618636,"about_ca_system_score_gemma":0.00011135899,"threshold_uncertainty_score":0.005237937},"labels":[],"label_agreement":null},{"id":"W4377023319","doi":"10.3847/1538-4357/acc38f","title":"The Low-temperature Corona in ESO 511−G030 Revealed by NuSTAR and XMM-Newton","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Science and Technology Facilities Council; Shanghai Municipal Education Commission; Fudan University; National Natural Science Foundation of China; Natural Science Foundation of Shanghai","keywords":"Physics; Corona (planetary geology); Astrophysics; Astronomy; Astrobiology","score_opus":0.00650672052768226,"score_gpt":0.22214725892818862,"score_spread":0.21564053840050637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377023319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978472,0.00019027678,0.00012251963,0.000049982715,0.000004310725,0.000004715543,0.00036748112,0.00006674484,0.0013467319],"genre_scores_gemma":[0.9982388,0.00005858601,0.0003148813,0.00006814664,0.00000820369,0.0000051077773,0.0009717854,0.000015544221,0.00031890642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987257,0.000010551711,0.000008667342,0.000041251067,0.000035087174,0.00003188572],"domain_scores_gemma":[0.9995289,0.000036774043,0.00021001382,0.00006336829,0.000054160842,0.000106753585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028572982,0.000298935,0.0003619244,0.0012402324,0.00037303314,0.0006041575,0.00031642753,0.00052761694,0.0008227198],"category_scores_gemma":[0.00049806567,0.00018800347,0.0003283566,0.0008152432,0.00024613473,0.0002812291,0.00058608013,0.00017856443,0.00046527563],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050099444,0.00008187117,0.92566556,0.000060848386,0.00012498932,0.0015248142,0.0005177011,0.001420787,0.05731824,0.00025403354,0.0015703719,0.010959743],"study_design_scores_gemma":[0.0000070377378,0.000027668691,0.99776304,0.0000068080485,0.000016955748,0.00017804661,0.00005599115,0.0006129629,0.0006255815,0.000034476103,0.0006666298,0.0000047754506],"about_ca_topic_score_codex":0.008262801,"about_ca_topic_score_gemma":0.017315293,"teacher_disagreement_score":0.008262801,"about_ca_system_score_codex":0.0007860397,"about_ca_system_score_gemma":0.00018995491,"threshold_uncertainty_score":0.016429424},"labels":[],"label_agreement":null},{"id":"W4377091103","doi":"10.3847/1538-4357/acc39d","title":"Machine Learning Applied to X-Ray Spectra: Separating Stars in Orion Nebula Cluster from Active Galactic Nuclei in CDFS","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Stars; Spectral line; Supernova; Active galactic nucleus; Chandra Deep Field South; Astronomy; Brightness; Orion Nebula; Galaxy; Star formation","score_opus":0.012486091801867823,"score_gpt":0.2448197241405975,"score_spread":0.23233363233872967,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377091103","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99740607,0.00008844721,0.0017243262,0.000073934956,0.000011462343,0.000007728711,0.00021341174,0.00012316706,0.00035148955],"genre_scores_gemma":[0.99631506,0.000023871591,0.0026711496,0.000016859985,0.000007354577,0.0000047561402,0.0007904959,0.000006514651,0.00016385071],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99974114,0.00006517809,0.000018096296,0.00009138363,0.00004492146,0.0000392715],"domain_scores_gemma":[0.9989863,0.00047292968,0.0001253387,0.00008926358,0.00019625004,0.00012992705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008575999,0.00050530507,0.00027810043,0.001379067,0.00037261497,0.0005751547,0.00063859957,0.000595257,0.0004792664],"category_scores_gemma":[0.0023104213,0.00013082207,0.00036901137,0.0007267011,0.00025665408,0.00042107367,0.000507518,0.00040192006,0.00019227296],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035908291,0.0003148266,0.6814746,0.00006320895,0.00015888002,0.00023445567,0.000157495,0.24221449,0.00506311,0.00024375675,0.0013739271,0.06834215],"study_design_scores_gemma":[0.000021208454,0.000061841936,0.1928389,0.00001525465,0.000025500412,0.0000664758,0.00017434348,0.80237144,0.0035740156,0.00039350108,0.0004437097,0.000013795301],"about_ca_topic_score_codex":0.018519612,"about_ca_topic_score_gemma":0.01481456,"teacher_disagreement_score":0.018519612,"about_ca_system_score_codex":0.00079549983,"about_ca_system_score_gemma":0.00033599383,"threshold_uncertainty_score":0.03682363},"labels":[],"label_agreement":null},{"id":"W4377104813","doi":"10.3847/1538-4357/acc38b","title":"Merger Signatures are Common, but not Universal, in Massive, Recently Quenched Galaxies at z ∼ 0.7","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Office of Science; New Mexico State University; National Astronomical Observatory of Japan; York University; Carnegie Mellon University; College of Engineering, Michigan State University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Harvard University; Yale University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; High Energy Accelerator Research Organization; Ohio State University; Research Corporation for Science Advancement; University of Portsmouth; Vanderbilt University; Pennsylvania Space Grant Consortium; National Aeronautics and Space Administration; Aspen Center for Physics; Academia Sinica; U.S. Department of Energy; Research Corporation for Scientific Advancement; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Galaxy formation and evolution; Billion years; Luminous infrared galaxy; Sky; Star formation; Stellar mass; Redshift","score_opus":0.010360292508079754,"score_gpt":0.2190313135093012,"score_spread":0.20867102100122142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4377104813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99934417,0.000037159516,0.000050937233,0.000010525899,6.018122e-7,0.0000013906997,0.00010264025,0.000011643465,0.00044087847],"genre_scores_gemma":[0.99971765,0.000013965401,0.000030406089,0.000005246329,0.0000016213666,7.3155604e-7,0.00015223458,0.0000016996783,0.00007632667],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984884,0.000013076418,0.000014139371,0.000036087524,0.00003875243,0.00004902935],"domain_scores_gemma":[0.99884355,0.00016230757,0.0005579608,0.000091404385,0.00010963915,0.00023510112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021831512,0.0000981183,0.00014594145,0.0014124151,0.0002329661,0.000659029,0.0002378277,0.00016435479,0.0018265975],"category_scores_gemma":[0.0011364893,0.00010891062,0.0001413883,0.00056620635,0.0005132268,0.0002661427,0.0004551805,0.00016164566,0.00030116312],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001251179,0.000013396982,0.98678327,0.00000594526,0.000013618546,0.00007282385,0.0001996667,0.00006531089,0.009352878,0.00011940896,0.000115464034,0.003133083],"study_design_scores_gemma":[0.0000013572011,0.000014703483,0.9992785,8.2863465e-7,0.0000028943352,0.000091716065,0.000073332696,0.00008078985,0.0003550217,0.000025133008,0.00007470422,0.000001040887],"about_ca_topic_score_codex":0.003925161,"about_ca_topic_score_gemma":0.0056564934,"teacher_disagreement_score":0.003925161,"about_ca_system_score_codex":0.00020922195,"about_ca_system_score_gemma":0.00008506286,"threshold_uncertainty_score":0.007804632},"labels":[],"label_agreement":null},{"id":"W4378070871","doi":"10.3847/1538-4357/acc1e3","title":"WALLABY Pilot Survey: H i in the Host Galaxy of a Fast Radio Burst","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Australian Research Council; Government of Western Australia; European Southern Observatory; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; College of Engineering, Michigan State University; Macquarie University; Jet Propulsion Laboratory; Science and Industry Endowment Fund; Centre National d’Etudes Spatiales; Commonwealth Scientific and Industrial Research Organisation; Australian Government; University of North Carolina at Chapel Hill; California Institute of Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Michigan State University; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Fast radio burst; Milky Way; Star formation; Stars; Dwarf galaxy","score_opus":0.025535502353134835,"score_gpt":0.24898444325177263,"score_spread":0.2234489408986378,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378070871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971334,0.000074722426,0.000084405554,0.000044069715,0.000004769616,0.000015685902,0.00081534503,0.000014242011,0.0018134146],"genre_scores_gemma":[0.9959441,0.00010083298,0.00032763646,0.0000590451,0.000015685477,0.000023012839,0.0017833231,0.000016145757,0.0017302958],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997812,0.000016084992,0.000008300162,0.000042927357,0.000045150813,0.000106330765],"domain_scores_gemma":[0.99919564,0.000052257346,0.00022156304,0.00006657193,0.000084984065,0.0003790777],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002909595,0.00026658105,0.0002636407,0.0011644524,0.0008446231,0.00064185367,0.0002645711,0.00024718433,0.0041036243],"category_scores_gemma":[0.00043743575,0.00020045716,0.00012344353,0.0009089343,0.00039432914,0.0003117667,0.0011981175,0.0003551409,0.0010312633],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042275238,0.00010049891,0.97054815,0.000029568186,0.00002770922,0.0008785115,0.0012867766,0.0000648905,0.011630814,0.0001684686,0.0028891934,0.011952651],"study_design_scores_gemma":[0.000006613385,0.000047971163,0.9971142,0.0000079166275,0.0000039315964,0.00016680403,0.00034135475,0.000048271988,0.00036759395,0.000013828692,0.0018787525,0.0000027782635],"about_ca_topic_score_codex":0.036126085,"about_ca_topic_score_gemma":0.07514328,"teacher_disagreement_score":0.036126085,"about_ca_system_score_codex":0.00044611865,"about_ca_system_score_gemma":0.0004119653,"threshold_uncertainty_score":0.071831584},"labels":[],"label_agreement":null},{"id":"W4378086476","doi":"10.3847/1538-4357/acb698","title":"On the Hunt for the Origins of the Orphan–Chenab Stream: Detailed Element Abundances with APOGEE and Gaia","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Aspen Center for Physics; Ohio State University; Max-Planck-Institut für Astrophysik; City University of New York; Flatiron Health; U.S. Department of Energy; Smithsonian Institution; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Globular cluster; Astrophysics; Metallicity; Milky Way; Stars; Galaxy; Galactic halo; Dwarf galaxy; Astronomy; Population; Galactic Center; Halo","score_opus":0.013486515933511713,"score_gpt":0.23236238513570412,"score_spread":0.2188758692021924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378086476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989869,0.00004885514,0.00006109328,0.000024449957,0.000001407983,0.0000032228038,0.0002675631,0.000005507595,0.0006008723],"genre_scores_gemma":[0.9983581,0.0000552098,0.00030199852,0.000030893814,0.0000036585689,0.0000034367074,0.0008882001,0.000008244012,0.00035018646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988925,0.0000117916825,0.0000055552914,0.000038790044,0.000028433042,0.00002609959],"domain_scores_gemma":[0.9996178,0.00003620734,0.00012680775,0.000038795053,0.00008042317,0.00009994689],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020184249,0.00016356651,0.00019379953,0.0012498517,0.00037411487,0.0006199787,0.00013467224,0.00013832423,0.0013257994],"category_scores_gemma":[0.00047025344,0.000105314626,0.00013779567,0.001039983,0.00025205186,0.00030061576,0.00055326225,0.00019805385,0.00032574718],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041886637,0.000011524738,0.9938951,0.0000043200585,0.000023927683,0.00006796299,0.00013181781,0.00004313478,0.0030357402,0.00006457191,0.0002329497,0.0024469711],"study_design_scores_gemma":[0.0000019088627,0.000007951009,0.99871397,0.0000027341475,0.0000071443465,0.000053935426,0.0001649513,0.00020893879,0.0002681666,0.00002234633,0.0005467005,0.0000013257849],"about_ca_topic_score_codex":0.025014305,"about_ca_topic_score_gemma":0.03582708,"teacher_disagreement_score":0.025014305,"about_ca_system_score_codex":0.00033957572,"about_ca_system_score_gemma":0.0002548708,"threshold_uncertainty_score":0.049737394},"labels":[],"label_agreement":null},{"id":"W4378225313","doi":"10.3847/1538-4357/acc582","title":"Streams on FIRE: Populations of Detectable Stellar Streams in the Milky Way and FIRE","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Milky Way; Physics; STREAMS; Astrophysics; Population; Galaxy; Astronomy; Galactic Center; Stellar population; Star formation","score_opus":0.01324295292734485,"score_gpt":0.22868264306145875,"score_spread":0.2154396901341139,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378225313","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999127,0.00002184537,0.0003481025,0.000020369116,0.0000012181591,0.000003688636,0.00015432083,0.000025702362,0.000297941],"genre_scores_gemma":[0.99903905,0.000016434607,0.00042970176,0.000011465341,0.0000021397059,0.0000052049554,0.0003348422,0.00001695811,0.00014423524],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980634,0.000051150153,0.000011349764,0.000061354964,0.000027174476,0.000042672513],"domain_scores_gemma":[0.99855953,0.00046573146,0.00034486933,0.00020032295,0.00012432392,0.0003053421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007655377,0.00032591211,0.0005559863,0.0005890005,0.00041139295,0.0009669809,0.0010108737,0.0005957326,0.0015161927],"category_scores_gemma":[0.0040411027,0.0003502771,0.00069021084,0.00044005387,0.00062776066,0.0008205328,0.00078324095,0.00037224963,0.00014430251],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005912642,0.00013042656,0.66397077,0.00004088147,0.0003269225,0.00027403006,0.00033205497,0.32141852,0.004895138,0.002540503,0.000434975,0.0050445357],"study_design_scores_gemma":[0.00020636397,0.00024349082,0.21594842,0.000021182414,0.00009591253,0.00017867048,0.00036339657,0.77637696,0.0036577377,0.0018957027,0.0009609597,0.00005117516],"about_ca_topic_score_codex":0.0087287,"about_ca_topic_score_gemma":0.0071220654,"teacher_disagreement_score":0.0087287,"about_ca_system_score_codex":0.00082186266,"about_ca_system_score_gemma":0.0003852757,"threshold_uncertainty_score":0.0173558},"labels":[],"label_agreement":null},{"id":"W4378225464","doi":"10.3847/1538-4357/acc32c","title":"Stellar-reddening-based Extinction Maps for Cosmological Applications","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Jet Propulsion Laboratory; National Institutes of Health; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Universidad Nacional Autónoma de México; Max-Planck-Institut für Astrophysik; Nuclear Safety and Security Commission; Ministério da Ciência, Tecnologia e Inovação; Queen's University; Gordon and Betty Moore Foundation; Queen's University Belfast; University of Oxford; Astrophysics Division; Durham University; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Los Alamos National Laboratory; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Extinction (optical mineralogy); Galaxy; Astronomy; Quasar; Young stellar object; Star formation","score_opus":0.014961982219374557,"score_gpt":0.2404732394018543,"score_spread":0.22551125718247975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378225464","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.66747975,0.00071969716,0.29768184,0.00034753556,0.000043657234,0.00008772908,0.011553941,0.010357701,0.0117282085],"genre_scores_gemma":[0.81761986,0.00014718292,0.1772904,0.000028613615,0.000026509413,0.00001785928,0.0037072068,0.00031138066,0.00085086556],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999081,0.000021350344,0.000006139582,0.000021115497,0.00003344165,0.000009758675],"domain_scores_gemma":[0.9985588,0.00030036015,0.0002716873,0.00027117736,0.00045868428,0.00013929719],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049316784,0.0002875526,0.00019573703,0.0018939449,0.0001625032,0.0007110057,0.00037241075,0.00017812892,0.0031634849],"category_scores_gemma":[0.0021771446,0.0001756618,0.0001664211,0.001696929,0.00009335009,0.000499632,0.00045740444,0.00024840506,0.00062868785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033935596,0.00033294427,0.43174657,0.00027164898,0.00032404682,0.00024021961,0.0003317399,0.059995383,0.062605746,0.009681436,0.011917405,0.42221355],"study_design_scores_gemma":[0.000045416542,0.00006757984,0.75620544,0.000057784968,0.000070982765,0.00025117144,0.00021722965,0.19019872,0.024611875,0.009372872,0.018834636,0.00006636322],"about_ca_topic_score_codex":0.0040781554,"about_ca_topic_score_gemma":0.00703266,"teacher_disagreement_score":0.0040781554,"about_ca_system_score_codex":0.00022634801,"about_ca_system_score_gemma":0.00023860631,"threshold_uncertainty_score":0.010582924},"labels":[],"label_agreement":null},{"id":"W4378225702","doi":"10.3847/1538-4357/accadf","title":"G 68-34: A Double-lined M-dwarf Eclipsing Binary in a Hierarchical Triple System","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Starspot; White dwarf; Exoplanet; Radial velocity; Photometry (optics); Spectrograph; Astronomy; Light curve; Binary star; Population; Spectral line; Stars","score_opus":0.021264796480628092,"score_gpt":0.25273002859207266,"score_spread":0.23146523211144457,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378225702","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993254,0.000013979252,0.000102031096,0.000022997941,0.0000031415111,0.0000026438715,0.00003617963,0.000011380171,0.00048231322],"genre_scores_gemma":[0.9995704,0.0000037056352,0.00018167357,0.000014673721,0.000002180954,7.9480844e-7,0.000079899226,0.0000023952546,0.0001443271],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993455,0.000005722882,0.0000037346879,0.000021162587,0.000015274763,0.000019625535],"domain_scores_gemma":[0.9998479,0.000011664876,0.000044872304,0.0000130921035,0.000010798118,0.00007161956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000722573,0.00018008258,0.00021054634,0.0005077394,0.00082696293,0.000371039,0.00020194257,0.00029318494,0.0015202486],"category_scores_gemma":[0.00024965918,0.00008186006,0.00009862654,0.00033789067,0.0002749001,0.00012377805,0.0005343138,0.00024944602,0.0005777965],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000546396,0.0002169077,0.88019854,0.000040754938,0.000053059044,0.011205984,0.00080405135,0.0011188535,0.08701485,0.0016874153,0.0016597484,0.01545338],"study_design_scores_gemma":[0.00005752565,0.00060050725,0.9550728,0.000017984568,0.000052612497,0.021339253,0.0011560551,0.007435163,0.006121866,0.0018543749,0.0062619876,0.000029833956],"about_ca_topic_score_codex":0.0028199137,"about_ca_topic_score_gemma":0.005811865,"teacher_disagreement_score":0.0028199137,"about_ca_system_score_codex":0.00029519625,"about_ca_system_score_gemma":0.00017631357,"threshold_uncertainty_score":0.0056069493},"labels":[],"label_agreement":null},{"id":"W4378234349","doi":"10.3847/1538-4357/acc843","title":"A Large Double-ring Disk Around the Taurus M Dwarf J04124068+2438157","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Science and Technology Council; National Natural Science Foundation of China; Natural Sciences and Engineering Research Council of Canada; European Commission; Nuclear Safety and Security Commission; Space Telescope Science Institute; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; California Institute of Technology; Gordon and Betty Moore Foundation; W. M. Keck Foundation","keywords":"Astrophysics; Debris disk; Planet; Physics; Photoevaporation; Millimeter; Submillimeter Array; RADIUS; Stars; Accretion (finance); Scale height; Astronomy; Protoplanetary disk; Planetary system; Star formation","score_opus":0.018378377473881824,"score_gpt":0.264163617337014,"score_spread":0.24578523986313217,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378234349","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987483,0.000045762794,0.00015484633,0.000020215277,0.00000314156,0.0000022952033,0.00022089033,0.000050716044,0.0007538972],"genre_scores_gemma":[0.99890196,0.00001898697,0.00047751566,0.000016032744,0.000008935283,0.0000042148963,0.00038598035,0.0000078839685,0.00017851831],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999962,0.00000308913,0.0000019420588,0.000014142643,0.0000075293965,0.000011346271],"domain_scores_gemma":[0.9999138,0.000008430414,0.000031596162,0.000012875654,0.000008811411,0.00002447493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000060710772,0.00012900257,0.00020358937,0.00043244925,0.00029557192,0.0002646372,0.00029862876,0.00024536552,0.0011139505],"category_scores_gemma":[0.00013321191,0.00010864891,0.00013636959,0.00029186273,0.00011464616,0.00014345151,0.00026578645,0.000114574235,0.00025058974],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005845002,0.00022750901,0.41069937,0.00010009494,0.00009132289,0.0028314292,0.0005015699,0.0019521764,0.54606754,0.000497886,0.003954783,0.032491796],"study_design_scores_gemma":[0.000020570662,0.000051017865,0.98874986,0.0000063874863,0.000018408746,0.00040906802,0.00010469185,0.0030513706,0.0063146083,0.00006117936,0.0012061116,0.0000067307205],"about_ca_topic_score_codex":0.0020778833,"about_ca_topic_score_gemma":0.0033134257,"teacher_disagreement_score":0.0020778833,"about_ca_system_score_codex":0.00020037347,"about_ca_system_score_gemma":0.00006272437,"threshold_uncertainty_score":0.0041315556},"labels":[],"label_agreement":null},{"id":"W4378470500","doi":"10.3847/1538-4357/acc9bc","title":"The Chemodynamical Nature of the Triangulum–Andromeda Overdensity","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Institut national des sciences de l'Univers; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Natural Sciences and Engineering Research Council of Canada; Agencia Nacional de Investigación y Desarrollo; Ministerio de Ciencia e Innovación; Centre National de la Recherche Scientifique; Korea Astronomy and Space Science Institute; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Ministère de l'Education Nationale, de l'Enseignement Supérieur et de la Recherche; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University of Hawai'i; Fundação de Amparo à Pesquisa do Estado de São Paulo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Science Foundation","keywords":"Physics; Astrophysics; Milky Way; Population; Andromeda; Stars; Halo; Thin disk; Stellar population; Astronomy; Thick disk; Galaxy; Star formation","score_opus":0.006077211511859349,"score_gpt":0.2215728531868032,"score_spread":0.21549564167494384,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4378470500","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980798,0.00012340915,0.00015024774,0.000028523526,0.0000016326868,0.0000041211306,0.00020404637,0.0000060301118,0.0014022037],"genre_scores_gemma":[0.9996326,0.000029526625,0.000094620904,0.000003461013,0.0000018351717,0.0000011491037,0.00013128709,0.0000023078942,0.00010319347],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998311,0.000025912786,0.0000070551637,0.000052431547,0.000039125684,0.00004441841],"domain_scores_gemma":[0.99934155,0.0000923415,0.00026309985,0.000057527348,0.00009721429,0.00014827948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018958579,0.00014874824,0.00017204022,0.0019136501,0.00055412273,0.0010613034,0.00041111946,0.00015898692,0.001753474],"category_scores_gemma":[0.0011303384,0.00010449366,0.00016948185,0.0014639045,0.0005472341,0.00040485742,0.00085473154,0.00016454687,0.00025470488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004305618,0.000010213338,0.9914231,0.00000834215,0.000030724037,0.00016033617,0.00046470822,0.00021045847,0.002573162,0.0005298959,0.00012248581,0.0044235867],"study_design_scores_gemma":[0.0000010349802,0.000008709462,0.99769837,0.000004013242,0.0000067756437,0.00021991842,0.000613005,0.00056511053,0.00023214926,0.000123376,0.0005235887,0.0000039263327],"about_ca_topic_score_codex":0.01540384,"about_ca_topic_score_gemma":0.017471412,"teacher_disagreement_score":0.01540384,"about_ca_system_score_codex":0.00054026564,"about_ca_system_score_gemma":0.00019632018,"threshold_uncertainty_score":0.030628324},"labels":[],"label_agreement":null},{"id":"W4379052700","doi":"10.3847/1538-4357/acc93a","title":"The ISM in the z = 6.9 Interacting Galaxies of SPT0311-58","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; University of British Columbia","funders":"National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Astronomy; Interstellar medium","score_opus":0.010752725837043741,"score_gpt":0.23944361115283488,"score_spread":0.22869088531579115,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379052700","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99947983,0.00001106141,0.000015583862,0.000013600086,6.40846e-7,0.0000016480942,0.00007041895,0.000005339357,0.0004018978],"genre_scores_gemma":[0.99937975,0.000010689388,0.00005422475,0.000019981833,0.0000015500924,0.0000035167257,0.0002993149,0.0000034312532,0.00022742314],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.000013146635,0.0000048610646,0.000041484876,0.000021943459,0.0000406852],"domain_scores_gemma":[0.99966264,0.000031148244,0.00008375401,0.000018461466,0.000031108906,0.00017284368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011009,0.00019364031,0.0002713892,0.0006868496,0.0005914777,0.0006746636,0.00034020678,0.00032139826,0.0017048313],"category_scores_gemma":[0.00034104346,0.00017449775,0.00015884767,0.00062666583,0.0002906246,0.00021684551,0.0008732574,0.00029396024,0.00058538397],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018211067,0.00010255142,0.9833575,0.000009031004,0.000033756292,0.00039558805,0.0012057496,0.00018215427,0.010253143,0.00016772613,0.00047421016,0.0036364312],"study_design_scores_gemma":[0.000006275888,0.000028951581,0.9985368,0.000001909267,0.000006603975,0.000116641706,0.00047143112,0.00037365875,0.00017450465,0.00003240179,0.00024865678,0.0000021819094],"about_ca_topic_score_codex":0.016671361,"about_ca_topic_score_gemma":0.016756961,"teacher_disagreement_score":0.016671361,"about_ca_system_score_codex":0.00047974562,"about_ca_system_score_gemma":0.00013580978,"threshold_uncertainty_score":0.033148646},"labels":[],"label_agreement":null},{"id":"W4379054741","doi":"10.3847/1538-4357/acb93a","title":"Modeling the 2022 τ-Herculid Outburst","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Rio Tinto (Canada); Espace pour la vie; Western University","funders":"Nuclear Safety and Security Commission; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; National Aeronautics and Space Administration","keywords":"Physics; Astronomy; Astrophysics; Astrobiology","score_opus":0.017157636997242265,"score_gpt":0.2333861614228106,"score_spread":0.21622852442556834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379054741","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9892497,0.00014448921,0.0031884692,0.00030594814,0.000042818592,0.000025949352,0.0014636755,0.00015409631,0.0054248758],"genre_scores_gemma":[0.99787414,0.000050586623,0.00059064286,0.000026667905,0.000008867334,0.000015258096,0.0005439552,0.000018531411,0.0008713802],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998815,0.000020912013,0.0000057295906,0.000032118965,0.000015045474,0.000044669294],"domain_scores_gemma":[0.9995229,0.00016923348,0.00009079069,0.00002550413,0.000070858936,0.00012068682],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004045895,0.0006950857,0.0005121893,0.00047322866,0.0005664326,0.0011078761,0.0011690152,0.0017426378,0.0028652493],"category_scores_gemma":[0.0013058479,0.00044656263,0.00067606376,0.00048633627,0.0004521904,0.0006192886,0.0006439197,0.0008094473,0.0003433417],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007285834,0.000050392813,0.016183164,0.000016968861,0.00002491116,0.00018249474,0.000028473756,0.9808625,0.00043501702,0.0008998731,0.00045171005,0.0007916456],"study_design_scores_gemma":[0.000017555798,0.000019737912,0.0038171844,0.000003886314,0.000010297614,0.000013356639,0.00003528018,0.99551684,0.00009694794,0.00018526631,0.00027605414,0.000007662921],"about_ca_topic_score_codex":0.1313456,"about_ca_topic_score_gemma":0.050965607,"teacher_disagreement_score":0.1313456,"about_ca_system_score_codex":0.0020769641,"about_ca_system_score_gemma":0.0011885364,"threshold_uncertainty_score":0.26116216},"labels":[],"label_agreement":null},{"id":"W4379467224","doi":"10.3847/1538-4357/acc93b","title":"A Tale of Three Dwarfs: No Extreme Cluster Formation in Extreme Star-forming Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Ontario College of Art and Design","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"myr; Physics; Astrophysics; Galaxy; Photometry (optics); Stars; Star cluster; Star formation; Astronomy; Galaxy cluster; Cluster (spacecraft); Dwarf galaxy; Open cluster","score_opus":0.028042499250689086,"score_gpt":0.22309975031014045,"score_spread":0.19505725105945138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379467224","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99760795,0.000039328777,0.0010451429,0.000118905424,0.000006383018,0.0000030833482,0.00011459094,0.00004696344,0.0010176356],"genre_scores_gemma":[0.99949193,0.0000067306732,0.00025494792,0.000027432758,0.0000017455282,0.0000018626826,0.0000849139,0.000007242676,0.00012314481],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998323,0.00002832355,0.000009002008,0.00006276655,0.000023267872,0.00004429148],"domain_scores_gemma":[0.9990484,0.00022595571,0.00010633028,0.00012837077,0.00008970437,0.00040124456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058488536,0.00013462538,0.00043941799,0.00043992844,0.0008002483,0.0010674527,0.0007400668,0.0005764604,0.002359002],"category_scores_gemma":[0.002020198,0.00014710723,0.00045476458,0.00033107563,0.0011178182,0.0006038478,0.0009311909,0.0005526809,0.00023223601],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011607343,0.00027519107,0.8261585,0.00008397513,0.00035486184,0.0011110386,0.0011585623,0.1242566,0.010923554,0.020058377,0.0022320182,0.012226609],"study_design_scores_gemma":[0.0002459367,0.0005027344,0.70747286,0.00004719351,0.0001738078,0.0005849534,0.0020589062,0.2520257,0.006017783,0.02749141,0.00325137,0.00012735518],"about_ca_topic_score_codex":0.011736036,"about_ca_topic_score_gemma":0.009222733,"teacher_disagreement_score":0.011736036,"about_ca_system_score_codex":0.00072180736,"about_ca_system_score_gemma":0.00036531792,"threshold_uncertainty_score":0.023335457},"labels":[],"label_agreement":null},{"id":"W4379468511","doi":"10.3847/1538-4357/acc8d7","title":"Search for Gravitational Waves from Scorpius X-1 in LIGO O3 Data with Corrected Orbital Ephemeris","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Japan Society for the Promotion of Science; National Science and Technology Council; Ministry of Science and ICT, South Korea; Istituto Nazionale di Fisica Nucleare; Ministerio de Ciencia e Innovación; Alliance de recherche numérique du Canada; Centre National de la Recherche Scientifique; Universitat de les Illes Balears; Govern de les Illes Balears; Academia Sinica; National Science Foundation; University of Washington; Science and Technology Facilities Council; National Research Foundation; Ministerio de Ciencia, Innovación y Universidades; Ministry of Education, Culture, Sports, Science and Technology","keywords":"Physics; Ephemeris; LIGO; Gravitational wave; Astronomy; Astrophysics; Satellite","score_opus":0.033560965318198195,"score_gpt":0.34554109681635226,"score_spread":0.31198013149815407,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379468511","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956722,0.000067186964,0.0014376522,0.00005711385,0.0000061854494,0.0000080750515,0.0014603497,0.000269711,0.0010214328],"genre_scores_gemma":[0.99400336,0.000032307016,0.0018674994,0.000021629588,0.0000091623615,0.000007745953,0.0037520481,0.00008015754,0.00022603146],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995272,0.00007857448,0.000028019638,0.00012228885,0.00013526373,0.00010871005],"domain_scores_gemma":[0.9985877,0.0003915451,0.00048190524,0.00024749571,0.00019940948,0.00009197841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00084369845,0.00036237633,0.0004213539,0.0016915576,0.00031955467,0.0007940468,0.00031981006,0.0002608352,0.0011169082],"category_scores_gemma":[0.0022040934,0.00016802388,0.00061055215,0.0018943353,0.0003248518,0.00035513358,0.00064902083,0.00043548734,0.00035468562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009272629,0.000104870385,0.91540974,0.000100965255,0.00049043243,0.00083707337,0.00036514958,0.018363992,0.02839953,0.0010286574,0.0034986162,0.03047374],"study_design_scores_gemma":[0.00006733303,0.000053625216,0.95630306,0.000016182797,0.00010548666,0.00019540454,0.000100107914,0.032655884,0.006541944,0.0003579461,0.003579318,0.00002382854],"about_ca_topic_score_codex":0.016409066,"about_ca_topic_score_gemma":0.013851079,"teacher_disagreement_score":0.016409066,"about_ca_system_score_codex":0.00042419237,"about_ca_system_score_gemma":0.00071978365,"threshold_uncertainty_score":0.032627106},"labels":[],"label_agreement":null},{"id":"W4379536992","doi":"10.3847/1538-4357/acc65f","title":"A Large-scale Magneto-ionic Fluctuation in the Local Environment of Periodic Fast Radio Burst Source FRB 20180916B","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Fast radio burst; Polarization (electrochemistry); Faraday effect; Astrophysics; Magnetic field; Neutron star","score_opus":0.008147931279138548,"score_gpt":0.26423956113784225,"score_spread":0.2560916298587037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4379536992","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99883085,0.00005905703,0.00008182571,0.000030668758,0.000003709885,0.0000024317287,0.0002810506,0.000016560072,0.00069383095],"genre_scores_gemma":[0.99886876,0.00002903003,0.00016089703,0.000014512973,0.000008652292,0.0000054527814,0.0006594825,0.000010886054,0.00024219799],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993443,0.000002885439,0.0000023550065,0.0000213424,0.000017097562,0.000021856978],"domain_scores_gemma":[0.9997861,0.000012872744,0.000084017964,0.000016040018,0.000040031216,0.00006098381],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011400241,0.00022115708,0.00023217777,0.0006323481,0.00042924468,0.00041368112,0.00031886811,0.00026075018,0.0010756965],"category_scores_gemma":[0.0003095061,0.00017527265,0.00011969042,0.00039244242,0.00024882294,0.00018865097,0.00038983437,0.0002408901,0.00033877834],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005640193,0.00007073956,0.6991623,0.000055059776,0.00006439853,0.0007776511,0.00053594715,0.0006236749,0.28633192,0.00019869296,0.0010551563,0.010560453],"study_design_scores_gemma":[0.000007850244,0.000022255163,0.997572,0.0000035870942,0.0000069125317,0.000108463166,0.00007420666,0.00040978836,0.0011764345,0.000023282231,0.000590831,0.0000043810896],"about_ca_topic_score_codex":0.009508029,"about_ca_topic_score_gemma":0.011556216,"teacher_disagreement_score":0.009508029,"about_ca_system_score_codex":0.00044989938,"about_ca_system_score_gemma":0.00016110801,"threshold_uncertainty_score":0.018905342},"labels":[],"label_agreement":null},{"id":"W4380047971","doi":"10.3847/1538-4357/acc8cd","title":"Unraveling Twisty Linear Polarization Morphologies in Black Hole Images","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Ministerio de Ciencia e Innovación; European Commission; Generalitat Valenciana; Space Telescope Science Institute; High Energy Physics; Gordon and Betty Moore Foundation; John Templeton Foundation; Office of International Science and Engineering; National Aeronautics and Space Administration; Harvard University; National Science Foundation","keywords":"Physics; Faraday effect; Magnetic field; Astrophysics; Computational physics; Polarization (electrochemistry); Black hole (networking); Linear polarization; Optics; Quantum mechanics","score_opus":0.020436521493368567,"score_gpt":0.2599783084718253,"score_spread":0.23954178697845674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380047971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98805016,0.000077460085,0.008581683,0.00023525575,0.000017839639,0.000026174075,0.00015275381,0.00020103541,0.0026576372],"genre_scores_gemma":[0.99775225,0.000028393602,0.0018298246,0.00002835853,0.000006361527,0.000007889568,0.00006218262,0.000047698857,0.00023708714],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998981,0.000029081262,0.0000029019247,0.000011240261,0.000015029144,0.00004374054],"domain_scores_gemma":[0.9993414,0.00028105697,0.000111541354,0.000076828335,0.00005904469,0.00013007515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049747614,0.00045159212,0.0005772813,0.0004429416,0.00046902816,0.00097375474,0.0006604708,0.000621275,0.0018012304],"category_scores_gemma":[0.0017738703,0.00032916336,0.0005247081,0.00026247997,0.00088526186,0.00077722524,0.0007197823,0.0005585992,0.00012139931],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021337555,0.00010427526,0.012572757,0.00005062819,0.00007668491,0.00038637375,0.0002227855,0.96477324,0.011794893,0.0069672284,0.00046959234,0.0023680138],"study_design_scores_gemma":[0.00003049034,0.000026946358,0.002093041,0.0000038879484,0.000005625443,0.000013282885,0.000039742674,0.99546164,0.0009686424,0.0012416525,0.00010713426,0.000007932844],"about_ca_topic_score_codex":0.0065017403,"about_ca_topic_score_gemma":0.0028182315,"teacher_disagreement_score":0.0065017403,"about_ca_system_score_codex":0.0007342551,"about_ca_system_score_gemma":0.0005096095,"threshold_uncertainty_score":0.012927771},"labels":[],"label_agreement":null},{"id":"W4380051478","doi":"10.3847/1538-4357/acc9b3","title":"LIMFAST. II. Line Intensity Mapping as a Probe of High-redshift Galaxy Formation","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Reionization; Astrophysics; Star formation; Astronomy; Galaxy; Redshift; Galaxy formation and evolution; Protogalaxy; Intensity mapping; Interacting galaxy; Lenticular galaxy","score_opus":0.012513737730569003,"score_gpt":0.21818816004431854,"score_spread":0.20567442231374955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380051478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88318205,0.00007267711,0.105309844,0.00020460506,0.000030122488,0.000034117922,0.0015265131,0.0046210485,0.005019096],"genre_scores_gemma":[0.97347057,0.00001979712,0.024721442,0.000052200467,0.000006567376,0.000032238844,0.00064671435,0.00027779446,0.00077263365],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985373,0.00006059071,0.0000034826598,0.000040773713,0.000022473707,0.000018941912],"domain_scores_gemma":[0.9992235,0.00039325783,0.00011878139,0.00014595709,0.000046796755,0.00007177614],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001011926,0.00029703582,0.00020435077,0.0002961445,0.00016167447,0.00044819427,0.00086651504,0.0003610711,0.0023901898],"category_scores_gemma":[0.0022847522,0.00021320932,0.000298017,0.00028415336,0.00032937338,0.00062857784,0.0007886236,0.00044825044,0.00026761266],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010411349,0.00025963344,0.14914112,0.00019751098,0.00027350982,0.00028839233,0.00026686687,0.72745943,0.046284698,0.02163199,0.0034880368,0.04966766],"study_design_scores_gemma":[0.000035985115,0.00014958392,0.015931001,0.000006300229,0.00001996043,0.00004881087,0.000035414992,0.967469,0.010351974,0.004502874,0.001430324,0.00001884447],"about_ca_topic_score_codex":0.0017207273,"about_ca_topic_score_gemma":0.0018571633,"teacher_disagreement_score":0.0023901898,"about_ca_system_score_codex":0.00038356136,"about_ca_system_score_gemma":0.00019918027,"threshold_uncertainty_score":0.007995963},"labels":[],"label_agreement":null},{"id":"W4380077593","doi":"10.3847/1538-4357/acca76","title":"Molecular Gas and Star Formation in Nearby Starburst Galaxy Mergers","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Star formation; Virial theorem; Sigma; Velocity dispersion; Stars; Galaxy merger; Spiral galaxy; Astronomy","score_opus":0.00699659370992937,"score_gpt":0.21051314158523454,"score_spread":0.20351654787530518,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380077593","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990689,0.00003187942,0.00062200194,0.00001957105,0.0000013621299,0.0000025353947,0.00004327703,0.000019987872,0.0001905868],"genre_scores_gemma":[0.9996655,0.000010629003,0.00023107146,0.0000039300426,0.0000011238626,0.0000016531484,0.000044789307,0.0000029681876,0.000038338138],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99991786,0.0000248382,0.000003840544,0.000021896549,0.000014528715,0.000017013966],"domain_scores_gemma":[0.99962485,0.00013492107,0.00011520025,0.0000361893,0.000025770998,0.00006301464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032228776,0.00031829375,0.000302417,0.0002743597,0.0002771388,0.00045756667,0.00060692255,0.0005319263,0.0006362434],"category_scores_gemma":[0.0009908085,0.0002049944,0.00043460008,0.0002782094,0.00032035355,0.0004530652,0.00042064098,0.00028119047,0.00006299784],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024429453,0.00014358528,0.16968255,0.000024336963,0.00012987804,0.00020643219,0.00009558759,0.81402606,0.01211984,0.0013075415,0.00012911743,0.0018907338],"study_design_scores_gemma":[0.000068873596,0.00020956127,0.081427656,0.0000044862895,0.000046530706,0.00009074908,0.00005597317,0.91385525,0.003275095,0.00072168,0.00022748183,0.00001671566],"about_ca_topic_score_codex":0.007545181,"about_ca_topic_score_gemma":0.0033355262,"teacher_disagreement_score":0.007545181,"about_ca_system_score_codex":0.00050471636,"about_ca_system_score_gemma":0.00019263446,"threshold_uncertainty_score":0.015002489},"labels":[],"label_agreement":null},{"id":"W4380354059","doi":"10.3847/1538-4357/accb56","title":"Heat Transport and Convective Velocities in Compositionally Driven Convection in Neutron Star and White Dwarf Interiors","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Heliophysics Division; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Convection; Convection zone; Convective heat transfer; Free convective layer; Astrophysics; Heat flux; Mechanics; Heat transfer","score_opus":0.007767165653213592,"score_gpt":0.21528638409994785,"score_spread":0.20751921844673427,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380354059","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990791,0.000041832427,0.00062332186,0.00000880539,0.0000015920153,0.0000018751712,0.000022964376,0.000012375197,0.00020821957],"genre_scores_gemma":[0.9995975,0.000013971969,0.00027253723,0.0000019679437,9.0611127e-7,0.0000016631355,0.000028826122,0.0000059070944,0.000076700424],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999386,0.00001304252,0.000004775391,0.000015644875,0.000014197163,0.000013798787],"domain_scores_gemma":[0.99975663,0.00010405791,0.00004972316,0.000017602308,0.00003744838,0.000034573997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003171485,0.0003127118,0.00033891093,0.00045379737,0.00032843833,0.0004369394,0.0002528985,0.0002652035,0.0003126283],"category_scores_gemma":[0.00089211436,0.00018221037,0.00032322132,0.00021069194,0.00053420896,0.00033682177,0.00039570552,0.00022671759,0.0000723179],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010672511,0.00015935743,0.14433064,0.000108953645,0.00013232604,0.0003135515,0.00054798945,0.3783955,0.4631498,0.0044147423,0.00015118395,0.0072286413],"study_design_scores_gemma":[0.00008244431,0.000177141,0.070728004,0.00001122694,0.000021852717,0.00007448337,0.00011529512,0.86426055,0.063017555,0.0011858149,0.00029191357,0.000033665616],"about_ca_topic_score_codex":0.0045613847,"about_ca_topic_score_gemma":0.0014750165,"teacher_disagreement_score":0.0045613847,"about_ca_system_score_codex":0.0006689988,"about_ca_system_score_gemma":0.00024025154,"threshold_uncertainty_score":0.009069681},"labels":[],"label_agreement":null},{"id":"W4380627117","doi":"10.3847/1538-4357/acbd44","title":"New Chondritic Bodies Identified in Eight Oxygen-bearing White Dwarfs","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"National Aeronautics and Space Administration","keywords":"White dwarf; Chondrite; Physics; Parent body; Meteorite; Astrobiology; Solar System; Astrophysics; Black dwarf; Oxygen; Astronomy; Stars","score_opus":0.012561603071102795,"score_gpt":0.22863025940592538,"score_spread":0.21606865633482258,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380627117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996352,0.000032879536,0.00010258352,0.0000019228983,0.0000012393018,0.0000032153876,0.00006157028,0.000005394645,0.00015596345],"genre_scores_gemma":[0.99902153,0.000034059492,0.00036554146,0.000006869097,0.0000036082135,0.000004091345,0.00033061675,0.0000034880943,0.00023017681],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998733,0.0000073417264,0.000013591083,0.000035506077,0.000036019846,0.000034315355],"domain_scores_gemma":[0.99967694,0.00003699986,0.0001061428,0.000036041838,0.00005810784,0.00008568051],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014736249,0.0001974693,0.000246258,0.0011923079,0.0003483335,0.00043758794,0.00018970872,0.00018908028,0.0006266491],"category_scores_gemma":[0.00030111344,0.00018439101,0.00017904076,0.0004763315,0.00024303395,0.00016975048,0.00062392507,0.00014452891,0.00023817991],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001385051,0.000027877788,0.9232557,0.000019656905,0.000022972597,0.0006631338,0.00047039278,0.00002835382,0.06866654,0.00003584409,0.00004722242,0.0066238227],"study_design_scores_gemma":[0.000004006639,0.00009053904,0.9917726,0.0000029128967,0.000014040162,0.0009867859,0.00021809974,0.00009595817,0.0061912197,0.000020385305,0.00060080766,0.0000026428982],"about_ca_topic_score_codex":0.0016823411,"about_ca_topic_score_gemma":0.003402703,"teacher_disagreement_score":0.0016823411,"about_ca_system_score_codex":0.0001365786,"about_ca_system_score_gemma":0.00010033909,"threshold_uncertainty_score":0.0033450723},"labels":[],"label_agreement":null},{"id":"W4380627449","doi":"10.3847/1538-4357/acc586","title":"Comparison of Polarized Radiative Transfer Codes Used by the EHT Collaboration","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; University of Waterloo; Canadian Institute for Advanced Research; McGill University","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; High Energy Physics; National Institutes of Natural Sciences; Science and Technology Facilities Council; National Nuclear Security Administration; Office of Science; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Instituto de Astrofísica de Andalucía; Recruitment Program of Global Experts; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; National Research Foundation of Korea; Chinese Academy of Sciences; National Key Research and Development Program of China; European Southern Observatory; Universiteit Leiden; Korea Astronomy and Space Science Institute; Toray Science Foundation; National Research Foundation; University of Pretoria; Radboud Universiteit; Vetenskapsrådet; Smithsonian Institution; John Templeton Foundation; National Radio Astronomy Observatory; U.S. Department of Energy; National Natural Science Foundation of China; Academia Sinica; Ministerio de Ciencia e Innovación; European Commission; Universiteit van Amsterdam; Gordon and Betty Moore Foundation; Ministerio de Ciencia, Innovación y Universidades; Fundação de Amparo à Pesquisa do Estado de São Paulo; University of Chicago; University of Arizona; Government of Canada; National Science Foundation","keywords":"Physics; Radiative transfer; Observable; Astrophysics; Supermassive black hole; Computational physics; Optics; Galaxy; Quantum mechanics","score_opus":0.023867849282903437,"score_gpt":0.29352317262443395,"score_spread":0.26965532334153053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380627449","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8546515,0.0004841812,0.080336295,0.0008113173,0.00030006736,0.00038129714,0.007876125,0.019506404,0.035652783],"genre_scores_gemma":[0.846755,0.00024317436,0.13178597,0.00022715054,0.00006707287,0.00035771547,0.013181548,0.005748441,0.0016339374],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99464417,0.0015531675,0.0004384672,0.00059056876,0.0021507784,0.00062287797],"domain_scores_gemma":[0.9815833,0.004987627,0.0009227511,0.0058932095,0.0058579315,0.0007551643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0077122436,0.001024671,0.0007464376,0.0018371335,0.00095303985,0.0023006804,0.0021922647,0.0012528636,0.0020418707],"category_scores_gemma":[0.022657122,0.0005781413,0.0012921577,0.0026194432,0.0008361939,0.0017417488,0.0022529992,0.0011579859,0.001095404],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.008410958,0.0010902389,0.10962169,0.000638004,0.0011667501,0.0011858948,0.0027553246,0.56619066,0.036123127,0.06198765,0.03720461,0.17362511],"study_design_scores_gemma":[0.0009820488,0.000477003,0.021236844,0.00011641201,0.00014614138,0.00035693194,0.00063121255,0.87576336,0.06753277,0.012331493,0.020200731,0.00022502326],"about_ca_topic_score_codex":0.007448986,"about_ca_topic_score_gemma":0.003250263,"teacher_disagreement_score":0.0077122436,"about_ca_system_score_codex":0.0014540062,"about_ca_system_score_gemma":0.0014307691,"threshold_uncertainty_score":0.040786743},"labels":[],"label_agreement":null},{"id":"W4380627497","doi":"10.3847/1538-4357/accde0","title":"Pulsar Double Lensing Sheds Light on the Origin of Extreme Scattering Events","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Ministry of Science and Technology, Taiwan; Simons Foundation; National Science Foundation","keywords":"Physics; Line-of-sight; Brightness; Lens (geology); Scattering; Astrophysics; Pulsar; Optics; Event (particle physics); Astronomy","score_opus":0.045685312301151484,"score_gpt":0.3330682906331093,"score_spread":0.2873829783319578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380627497","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9846097,0.0002670788,0.010913622,0.00023307363,0.000025860321,0.000005245207,0.00008355938,0.0001904368,0.0036714901],"genre_scores_gemma":[0.99852544,0.00005473001,0.0011718774,0.000013523703,0.000014130153,0.0000013141661,0.000025307083,0.0000132956775,0.00018036213],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999399,0.000009353225,0.0000032569326,0.000016448817,0.0000146830935,0.000016408567],"domain_scores_gemma":[0.99942183,0.00019031604,0.00018187278,0.00012061962,0.000031591368,0.000053738888],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017620702,0.0003191902,0.00027042732,0.0004140399,0.0003633051,0.0007025104,0.00021537508,0.00052691984,0.0012006613],"category_scores_gemma":[0.00056271476,0.0002199647,0.00024578156,0.00030495037,0.00068562856,0.0008404252,0.00064689555,0.00065121864,0.00019911648],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010402143,0.00012485917,0.20211834,0.00017573792,0.00011977224,0.0063301083,0.0009501571,0.026492348,0.61687297,0.07733245,0.0030977463,0.06534532],"study_design_scores_gemma":[0.00014431977,0.0003790972,0.5281111,0.000050215345,0.00011572169,0.008635823,0.0010067801,0.22818166,0.15914656,0.061681375,0.012352362,0.0001949513],"about_ca_topic_score_codex":0.00064118934,"about_ca_topic_score_gemma":0.00042017872,"teacher_disagreement_score":0.0012006613,"about_ca_system_score_codex":0.00027196397,"about_ca_system_score_gemma":0.00006699443,"threshold_uncertainty_score":0.004016638},"labels":[],"label_agreement":null},{"id":"W4380630126","doi":"10.3847/1538-4357/acd04c","title":"Gemini Near Infrared Spectrograph–Distant Quasar Survey: Augmented Spectroscopic Catalog and a Prescription for Correcting UV-based Quasar Redshifts","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Quasar; Spectrograph; Redshift; Astrophysics; Astronomy; Infrared; OVV quasar; Red shift; Spectral line; Galaxy","score_opus":0.015089438948641919,"score_gpt":0.24407753828499185,"score_spread":0.22898809933634992,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380630126","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7841189,0.0003724729,0.14699298,0.00032147518,0.00006586577,0.0005205035,0.04650311,0.013909393,0.007195321],"genre_scores_gemma":[0.6271527,0.00019298343,0.31065047,0.00013806236,0.00007142253,0.00046630096,0.05743644,0.0005963847,0.0032952707],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99868566,0.00031751962,0.00018126368,0.00034435873,0.00038111987,0.00009001409],"domain_scores_gemma":[0.9958497,0.00036983998,0.001232258,0.0014134067,0.0010297443,0.00010503302],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0036276283,0.00067374797,0.0004429169,0.0024408079,0.0005509172,0.00092634244,0.0010366787,0.0004906099,0.0022704643],"category_scores_gemma":[0.0063960617,0.0004896545,0.0004211457,0.001794353,0.00022888914,0.0004659387,0.000848413,0.00038629607,0.0019734022],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024925795,0.00022650954,0.8368021,0.00015547313,0.00015921047,0.000083564955,0.00029397281,0.021402288,0.018499976,0.0021825193,0.016104436,0.10384063],"study_design_scores_gemma":[0.000063873944,0.00010463967,0.8803323,0.00004063096,0.000102432634,0.00012315148,0.00009147748,0.07810858,0.014613475,0.0005809053,0.025788,0.00005049078],"about_ca_topic_score_codex":0.019278992,"about_ca_topic_score_gemma":0.03187946,"teacher_disagreement_score":0.019278992,"about_ca_system_score_codex":0.00080710894,"about_ca_system_score_gemma":0.0010468359,"threshold_uncertainty_score":0.038333595},"labels":[],"label_agreement":null},{"id":"W4380630411","doi":"10.3847/1538-4357/acd04d","title":"Shedding New Light on Weak Emission-line Quasars in the C iv–Hβ Parameter Space","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"HORIZON EUROPE European Research Council; Israel Science Foundation; National Natural Science Foundation of China; European Commission; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Quasar; Astrophysics; Line (geometry); Emission spectrum; Space (punctuation); Parameter space; Astronomy; Spectral line; Galaxy; Geometry","score_opus":0.013403951261544308,"score_gpt":0.2492680847187282,"score_spread":0.23586413345718388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380630411","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962482,0.00068821333,0.0015430691,0.0003271235,0.000012946699,0.0000021885112,0.00014700538,0.000014326385,0.001016962],"genre_scores_gemma":[0.99905163,0.00019261811,0.0004101685,0.00010270968,0.00006302862,0.0000011316816,0.000084167164,0.000008280267,0.00008619165],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997261,0.000083148494,0.000019474635,0.00006512274,0.000060449485,0.00004569764],"domain_scores_gemma":[0.99520314,0.0022328466,0.0015113096,0.00048698395,0.00018653081,0.0003792288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011167444,0.0002821411,0.00037497788,0.00118322,0.00023569247,0.0015701305,0.0003785433,0.00041243192,0.0018981654],"category_scores_gemma":[0.003638314,0.00016097778,0.00019728488,0.0010733436,0.00086972374,0.0017019673,0.0007777787,0.00069781725,0.00017282976],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008756295,0.00005948074,0.96609515,0.000046014247,0.0000881339,0.00029896005,0.00045976503,0.00086593133,0.006917957,0.0021050884,0.00076565595,0.022210348],"study_design_scores_gemma":[0.000007611618,0.00006290566,0.98940456,0.000020535814,0.000022295922,0.0003630779,0.00088908925,0.0025497419,0.0007382332,0.003658282,0.002265454,0.000018109075],"about_ca_topic_score_codex":0.0015395435,"about_ca_topic_score_gemma":0.002672983,"teacher_disagreement_score":0.0018981654,"about_ca_system_score_codex":0.00013056384,"about_ca_system_score_gemma":0.00012168905,"threshold_uncertainty_score":0.006349981},"labels":[],"label_agreement":null},{"id":"W4380632280","doi":"10.3847/1538-4357/acd0af","title":"X-Ray Polarimetry of the Accreting Pulsar 1A 0535+262 in the Supercritical State with PolarLight","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Key Research and Development Program of China; National Natural Science Foundation of China","keywords":"Pulsar; Physics; Astrophysics; Polarimetry; Supercritical fluid; Neutron star; Polarization (electrochemistry); Astronomy; Scattering; Optics","score_opus":0.011002344492490353,"score_gpt":0.2353513657510633,"score_spread":0.22434902125857295,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380632280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982836,0.00008612285,0.00032989113,0.000014068757,0.000002523371,0.000003922111,0.000102947546,0.000020880365,0.00115612],"genre_scores_gemma":[0.9993414,0.000030198147,0.00028504798,0.000009670103,0.0000036453143,0.0000028137958,0.0001426852,0.0000033501378,0.00018115813],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999299,0.000009018655,0.000003737225,0.000018682847,0.000020790409,0.000017997609],"domain_scores_gemma":[0.9998634,0.00002141975,0.000045214507,0.000017429884,0.000023614319,0.000029015599],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016142894,0.00016152023,0.0001009079,0.00072262425,0.00028032722,0.00050209183,0.00016747124,0.00016166522,0.0006635038],"category_scores_gemma":[0.0002678107,0.00011638142,0.00008402977,0.0004362741,0.00029090486,0.00022473391,0.00033656307,0.0002603455,0.00011080616],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00054977543,0.000062928666,0.20221125,0.000046261022,0.00004466206,0.00048847863,0.00039740748,0.0008256685,0.7832714,0.0008867178,0.00040793978,0.010807581],"study_design_scores_gemma":[0.00003163699,0.00026472638,0.8784411,0.000012782014,0.000033410033,0.00047977766,0.00023301075,0.0029036005,0.11485557,0.00033561452,0.0023902878,0.000018512887],"about_ca_topic_score_codex":0.001710024,"about_ca_topic_score_gemma":0.0022370908,"teacher_disagreement_score":0.001710024,"about_ca_system_score_codex":0.00019565922,"about_ca_system_score_gemma":0.000098674886,"threshold_uncertainty_score":0.0034000874},"labels":[],"label_agreement":null},{"id":"W4380685735","doi":"10.3847/1538-4357/accf8f","title":"Sparse Logistic Regression for RR Lyrae versus Binaries Classification","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"HORIZON EUROPE Marie Sklodowska-Curie Actions; Ministero dell'Università e della Ricerca","keywords":"Light curve; Physics; RR Lyrae variable; Astrophysics; Artificial intelligence; Logistic regression; Classifier (UML); Stars; Pattern recognition (psychology); Machine learning; Computer science","score_opus":0.0770172038871441,"score_gpt":0.30335772077264794,"score_spread":0.22634051688550383,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380685735","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8066546,0.002369071,0.17302144,0.0018111782,0.00028821087,0.0001550768,0.0039683837,0.007139239,0.0045929584],"genre_scores_gemma":[0.9669611,0.00013931993,0.025642578,0.00016396123,0.00012347924,0.00005642503,0.004760663,0.00010349568,0.0020490983],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9983871,0.00061178854,0.00009525457,0.00045949564,0.00023381825,0.00021255638],"domain_scores_gemma":[0.9966068,0.0017476785,0.00032135163,0.0004911857,0.0006756745,0.00015730073],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027645323,0.0011029568,0.0008274635,0.0016586849,0.00037548906,0.00082148175,0.0011186028,0.0010861296,0.0015006592],"category_scores_gemma":[0.008207271,0.00019920763,0.00078610406,0.0010448423,0.00038256423,0.0006215303,0.0011360461,0.0012946367,0.0014390066],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010768288,0.0006552615,0.07639446,0.00023638037,0.00032975717,0.00032882162,0.00016200186,0.44860432,0.00881618,0.0019337387,0.0275223,0.43393993],"study_design_scores_gemma":[0.000015003519,0.00003684242,0.004030131,0.000012390453,0.00001139802,0.00002346389,0.000030020508,0.99296933,0.0014246536,0.00070840196,0.0007295975,0.000008849384],"about_ca_topic_score_codex":0.007099281,"about_ca_topic_score_gemma":0.004230296,"teacher_disagreement_score":0.007099281,"about_ca_system_score_codex":0.0006173807,"about_ca_system_score_gemma":0.0005501534,"threshold_uncertainty_score":0.014620423},"labels":[],"label_agreement":null},{"id":"W4380885340","doi":"10.3847/1538-4357/acce3d","title":"The GeMS/GSAOI Galactic Globular Cluster Survey (G4CS). II. Characterization of 47 Tuc with Bayesian Statistics","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Fondo Nacional de Desarrollo Científico y Tecnológico","keywords":"Physics; Globular cluster; Astrophysics; Distance modulus; Photometry (optics); Milky Way; Astronomy; Galaxy; Star cluster; Markov chain Monte Carlo; Open cluster; Monte Carlo method; Stars; Statistics","score_opus":0.009919043941853582,"score_gpt":0.2224037370194389,"score_spread":0.21248469307758533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380885340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9219092,0.00042417157,0.043553688,0.00019940562,0.000014040839,0.00012445636,0.022948122,0.0017236024,0.009103217],"genre_scores_gemma":[0.9429779,0.00012408549,0.03281839,0.000052446438,0.000022114862,0.00006408436,0.022360694,0.000340561,0.0012396337],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996082,0.00009352875,0.000022910566,0.00011076709,0.000115459334,0.000049191378],"domain_scores_gemma":[0.99897397,0.0002643751,0.00026296143,0.00018432189,0.00020849054,0.000105842315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014192802,0.00028910217,0.0003659903,0.0028430193,0.000371644,0.00071437174,0.00060337316,0.00034321932,0.0019120714],"category_scores_gemma":[0.0035537651,0.00028193917,0.00050852716,0.0021857666,0.00034725873,0.00042565586,0.0005938154,0.00028740815,0.00081234606],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002157876,0.000044964974,0.8525078,0.00009715149,0.00016606123,0.00015334428,0.00026269854,0.058842443,0.008771442,0.005361366,0.01047439,0.063102484],"study_design_scores_gemma":[0.000040220773,0.000046690962,0.7377619,0.000044258803,0.000060928793,0.00014033743,0.00013373645,0.24218349,0.0034895546,0.006203673,0.009857075,0.000038071586],"about_ca_topic_score_codex":0.043006755,"about_ca_topic_score_gemma":0.043391258,"teacher_disagreement_score":0.043006755,"about_ca_system_score_codex":0.001150528,"about_ca_system_score_gemma":0.0006554992,"threshold_uncertainty_score":0.08551282},"labels":[],"label_agreement":null},{"id":"W4380992585","doi":"10.3847/1538-4357/accf89","title":"Subarcminute Localization of 13 Repeating Fast Radio Bursts Detected by CHIME/FRB","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":57,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; University of British Columbia; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; McGill Space Institute; Natural Sciences and Engineering Research Council of Canada; Instituto de Astrofísica de Canarias; University of Toronto; Canada Research Chairs; National Defense Science and Engineering Graduate; Smithsonian Astrophysical Observatory; U.S. Department of Defense; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Fast radio burst; Galaxy","score_opus":0.009694011717869882,"score_gpt":0.28720961415775015,"score_spread":0.27751560243988027,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380992585","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960639,0.00016983281,0.0019694557,0.00002301868,0.0000069999237,0.000010429548,0.0005251448,0.00014415078,0.0010870808],"genre_scores_gemma":[0.99593604,0.000044611745,0.0028290437,0.000015374137,0.000007971571,0.0000075434677,0.0007985047,0.00002488764,0.00033615992],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998305,0.000013478812,0.0000057100756,0.00005209826,0.000045648183,0.00005248935],"domain_scores_gemma":[0.99946326,0.00007308464,0.00013843417,0.00009835681,0.00010244007,0.00012434438],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030179345,0.00023362382,0.00029786048,0.0012571615,0.00025250672,0.00033851343,0.00029799083,0.00027173277,0.0010925782],"category_scores_gemma":[0.0006490388,0.0001663148,0.00017855439,0.00058553607,0.00019893145,0.00015402227,0.0004902469,0.00028964123,0.00038211883],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008445511,0.00009499515,0.61308753,0.000085737185,0.00015725975,0.0015957478,0.000617299,0.0015668424,0.30707648,0.00027496988,0.0006974344,0.0739011],"study_design_scores_gemma":[0.000013409879,0.00009809105,0.98461837,0.0000056369167,0.000029604846,0.0005859075,0.00009082829,0.0013611023,0.01153991,0.0000677081,0.0015750736,0.000014310099],"about_ca_topic_score_codex":0.0031507786,"about_ca_topic_score_gemma":0.006280679,"teacher_disagreement_score":0.0031507786,"about_ca_system_score_codex":0.00026565194,"about_ca_system_score_gemma":0.000117144096,"threshold_uncertainty_score":0.006264925},"labels":[],"label_agreement":null},{"id":"W4380997943","doi":"10.3847/1538-4357/accb86","title":"The Physical Drivers and Observational Tracers of CO-to-H<sub>2</sub> Conversion Factor Variations in Nearby Barred Galaxy Centers","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":47,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Science Council; National Science and Technology Council; National Astronomical Observatory of Japan; Agencia Estatal de Investigación; National Radio Astronomy Observatory; European Regional Development Fund; Canadian Institute for Theoretical Astrophysics; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Velocity dispersion; Order (exchange); Line (geometry); Optical depth; Geometry","score_opus":0.013368180542139917,"score_gpt":0.22793244359045367,"score_spread":0.21456426304831375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4380997943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986547,0.000037029382,0.0003798017,0.0000427684,8.0377635e-7,0.0000029022576,0.0002590441,0.000017184415,0.0006057045],"genre_scores_gemma":[0.99966073,0.0000078190815,0.0000957534,0.000006184176,0.0000021718479,0.0000012333086,0.00017820722,0.000004335462,0.000043665146],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998142,0.000032806514,0.000009535157,0.00007293021,0.000041614978,0.00002896123],"domain_scores_gemma":[0.99784243,0.00042087698,0.0009851704,0.00022216563,0.00018559289,0.00034374083],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004774805,0.00012422311,0.00020869637,0.00092861487,0.00031213605,0.0008391484,0.00042129046,0.00027177474,0.0014816497],"category_scores_gemma":[0.0020902208,0.00023653872,0.00018400306,0.00081874296,0.0006689209,0.0006859011,0.0005480468,0.00035786233,0.000271979],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007819816,0.000028856824,0.9904171,0.0000070291076,0.00002935467,0.00005432531,0.0002376154,0.0008707278,0.0056708725,0.00066983816,0.00012052551,0.0018154468],"study_design_scores_gemma":[0.0000020026164,0.000005617891,0.9973482,0.0000016662055,0.0000038222374,0.000016232205,0.00010201565,0.0019156132,0.00032300365,0.00017020885,0.000108335254,0.0000033060037],"about_ca_topic_score_codex":0.015888294,"about_ca_topic_score_gemma":0.014513637,"teacher_disagreement_score":0.015888294,"about_ca_system_score_codex":0.00060830143,"about_ca_system_score_gemma":0.00015811567,"threshold_uncertainty_score":0.031591654},"labels":[],"label_agreement":null},{"id":"W4381432316","doi":"10.3847/1538-4357/acd2d0","title":"VERITAS Discovery of Very High Energy Gamma-Ray Emission from S3 1227+25 and Multiwavelength Observations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Science and Technology Facilities Council; U.S. Department of Energy; California Institute of Technology; European Commission; National Energy Research Scientific Computing Center; Nuclear Safety and Security Commission; Space Telescope Science Institute; Astrophysics Science Division; Office of Science; National Aeronautics and Space Administration; Aalto-Yliopisto; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Science Foundation","keywords":"Physics; High energy; Astrophysics; Gamma ray; Astronomy; Gamma-ray astronomy; Atomic physics","score_opus":0.01294982969530653,"score_gpt":0.2136186435136172,"score_spread":0.20066881381831067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4381432316","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99584323,0.00018062904,0.0004130596,0.000048313974,0.0000140519505,0.000011354932,0.00061989855,0.00008812691,0.0027813858],"genre_scores_gemma":[0.99803513,0.00003508588,0.00068474596,0.000029588018,0.000011670586,0.000005644754,0.00076503353,0.000014465971,0.00041849972],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997969,0.000014106811,0.000007787118,0.000051214687,0.00008528088,0.000044690656],"domain_scores_gemma":[0.9995976,0.00002695745,0.00014406178,0.0000454117,0.000044818054,0.00014115011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031872737,0.00030927843,0.0002637176,0.0008422706,0.00043007534,0.0007221709,0.0004192077,0.0003645628,0.0016025862],"category_scores_gemma":[0.00029366638,0.00019096369,0.00040042514,0.00057046494,0.00023728595,0.00014530285,0.000482616,0.00037010884,0.0004917568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00095168984,0.00017660453,0.70439774,0.00012243952,0.00030154292,0.0044203755,0.0005350601,0.0010953506,0.2593143,0.0011229491,0.0030730902,0.02448881],"study_design_scores_gemma":[0.00004170539,0.00025131647,0.98089373,0.000023129216,0.00005487662,0.0015429789,0.00013443445,0.0016570893,0.009625583,0.00025489315,0.005494174,0.000026064763],"about_ca_topic_score_codex":0.00488389,"about_ca_topic_score_gemma":0.017387008,"teacher_disagreement_score":0.00488389,"about_ca_system_score_codex":0.0006359654,"about_ca_system_score_gemma":0.00028684258,"threshold_uncertainty_score":0.009710908},"labels":[],"label_agreement":null},{"id":"W4381433428","doi":"10.3847/1538-4357/acd249","title":"Fading AGNs in Poststarburst Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Luminous infrared galaxy; Luminosity; Active galactic nucleus; Star formation; Astronomy; Radio galaxy; Doubly ionized oxygen; Emission spectrum; Spectral line","score_opus":0.01053538801279133,"score_gpt":0.2261915637879057,"score_spread":0.21565617577511437,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4381433428","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99840695,0.00009757885,0.00018450298,0.00002116674,0.0000032598014,0.000003195273,0.000116590956,0.000017262564,0.0011494736],"genre_scores_gemma":[0.99956363,0.000024061925,0.000071721464,0.000008728724,0.0000049299756,8.914786e-7,0.00010767981,0.0000018043277,0.00021651646],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985254,0.0000091957245,0.000008343453,0.000044902652,0.00003635502,0.000048589925],"domain_scores_gemma":[0.9981213,0.00022488245,0.0010178336,0.00013639525,0.00018203566,0.0003175491],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025956155,0.000121901816,0.00013588906,0.00092706113,0.000279351,0.00060429744,0.00024955426,0.00019537212,0.0026688157],"category_scores_gemma":[0.0009301841,0.00010118733,0.00015985216,0.00041412146,0.0003810359,0.00027327475,0.00037623223,0.00035775625,0.0003297155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009954163,0.000024571074,0.98034006,0.000011533586,0.00001419328,0.0002119894,0.0002449379,0.0001689624,0.009754699,0.00013021623,0.00014210405,0.008857195],"study_design_scores_gemma":[9.836671e-7,0.000023930868,0.9991054,0.0000013860475,0.000002462325,0.00016068273,0.000041934905,0.000108781234,0.0003190195,0.00003250562,0.00020170357,0.0000011792595],"about_ca_topic_score_codex":0.004451261,"about_ca_topic_score_gemma":0.004905934,"teacher_disagreement_score":0.004451261,"about_ca_system_score_codex":0.00032711338,"about_ca_system_score_gemma":0.00007585997,"threshold_uncertainty_score":0.00892812},"labels":[],"label_agreement":null},{"id":"W4381800561","doi":"10.3847/1538-4357/acc943","title":"Spectroscopic Analysis of Milky Way Outer Halo Satellites: Aquarius II and Boötes II","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; European Space Agency; National Science Foundation","keywords":"Physics; Metallicity; Astrophysics; Milky Way; Galaxy; Radial velocity; RR Lyrae variable; Velocity dispersion; Stellar kinematics; Stars; Dwarf galaxy; Local Group; Halo; Proper motion; Astronomy; Globular cluster","score_opus":0.01161643386555972,"score_gpt":0.23670978674642415,"score_spread":0.22509335288086443,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4381800561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982358,0.000033673958,0.00011174624,0.000011013769,0.0000013498156,0.0000034102152,0.0003393153,0.000017003627,0.0012467026],"genre_scores_gemma":[0.99750346,0.000023651737,0.00040312155,0.000012095572,0.000004394702,0.0000033770982,0.0013645713,0.000008701626,0.00067654887],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998723,0.000011816766,0.0000070831225,0.000041934487,0.000036033074,0.00003085866],"domain_scores_gemma":[0.9996321,0.000025937221,0.000111079906,0.000045390407,0.00006907943,0.000116314084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014123213,0.0002159873,0.00012373202,0.0013753565,0.0002704601,0.00036253218,0.00017046416,0.00009316947,0.0010812742],"category_scores_gemma":[0.000356708,0.00009570743,0.00010273165,0.0007299563,0.00020178879,0.00020369016,0.00057346246,0.00009440498,0.00021791978],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011785009,0.000027582277,0.9708241,0.000013191354,0.000033097847,0.00011458284,0.0002920124,0.00047883118,0.017447563,0.00022286136,0.0003902445,0.010038],"study_design_scores_gemma":[0.0000057205216,0.000030569143,0.99422294,0.0000033617284,0.0000087521685,0.000095235795,0.00023670925,0.00069758744,0.0025689742,0.00005563978,0.0020702905,0.0000043057235],"about_ca_topic_score_codex":0.00678351,"about_ca_topic_score_gemma":0.012017565,"teacher_disagreement_score":0.00678351,"about_ca_system_score_codex":0.00036478965,"about_ca_system_score_gemma":0.00008798285,"threshold_uncertainty_score":0.013488054},"labels":[],"label_agreement":null},{"id":"W4382450809","doi":"10.3847/1538-4357/accbc3","title":"Investigating the M <sub>GCS</sub>–M <sub> h </sub> Relation in the Most Massive Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Virial mass; Galaxy; Globular cluster; Dark matter; Halo; Astronomy; Galaxy cluster; Effective radius; Galaxy groups and clusters; Galaxy formation and evolution; Population; Medicine","score_opus":0.010849693938603445,"score_gpt":0.21285782277396417,"score_spread":0.20200812883536073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382450809","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99898094,0.000084176376,0.00014451475,0.000021661495,7.980497e-7,0.0000013988495,0.00011294378,0.0000056503454,0.00064777955],"genre_scores_gemma":[0.99974185,0.000014826525,0.00007065525,0.000005823202,0.0000027463507,6.226658e-7,0.00007832602,0.0000013710287,0.00008381562],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998821,0.000020266985,0.000007731851,0.000039354236,0.000021547321,0.00002890109],"domain_scores_gemma":[0.99857783,0.0004318418,0.0004887141,0.00012809534,0.00013387152,0.00023964228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033248062,0.00011727733,0.00015195027,0.0012948969,0.0002836707,0.0006291769,0.00020266284,0.00026303888,0.0013834718],"category_scores_gemma":[0.0013459219,0.00011124903,0.00012595502,0.0009259568,0.00040886665,0.00037147538,0.0005083101,0.00024365645,0.00039686603],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000021316782,0.0000061318838,0.9969367,0.0000031182337,0.000012098515,0.000020193913,0.00006966897,0.000075731485,0.0016392466,0.0001140564,0.000036878737,0.0010649968],"study_design_scores_gemma":[3.6971738e-7,0.0000086803175,0.9993717,7.182746e-7,0.0000036957938,0.000022605675,0.00007287819,0.0001420927,0.0002353989,0.000050598952,0.000090743015,5.264821e-7],"about_ca_topic_score_codex":0.0048381495,"about_ca_topic_score_gemma":0.0078019938,"teacher_disagreement_score":0.0048381495,"about_ca_system_score_codex":0.00026149006,"about_ca_system_score_gemma":0.00012634307,"threshold_uncertainty_score":0.009619951},"labels":[],"label_agreement":null},{"id":"W4382466934","doi":"10.3847/1538-4357/accf84","title":"Pixelated Reconstruction of Foreground Density and Background Surface Brightness in Gravitational Lensing Systems Using Recurrent Inference Machines","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; Fonds de recherche du Québec","keywords":"Physics; Gravitational lens; Artificial intelligence; Inference; Strong gravitational lensing; Parametric statistics; Mass distribution; Lens (geology); Galaxy; Computer vision; Weak gravitational lensing; Artificial neural network; Surface brightness; Convolutional neural network; Brightness; Parametric model; Astrophysics; Redshift; Computer science; Optics","score_opus":0.023749976322883636,"score_gpt":0.2590238262225723,"score_spread":0.23527384989968866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382466934","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.20925869,0.00022738644,0.7882315,0.00033842746,0.000026666272,0.000019507434,0.00009566741,0.0005699222,0.0012322712],"genre_scores_gemma":[0.9555352,0.00006875677,0.043083634,0.00005483864,0.000020792895,0.000021623766,0.00011049317,0.000046247387,0.0010583797],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998273,0.00006483095,0.000008117448,0.000046040997,0.00002792059,0.000025849256],"domain_scores_gemma":[0.9986268,0.0009186322,0.00017533112,0.00008605088,0.00013197973,0.000061190076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00093979033,0.0006395896,0.0008111054,0.0004215789,0.00027192506,0.0007579033,0.0012200641,0.001001532,0.0008715401],"category_scores_gemma":[0.004005957,0.00060338405,0.00053741544,0.00029231413,0.00082763616,0.0009032294,0.0006633675,0.00087776425,0.00014602303],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003934496,0.000012321265,0.00081405905,0.000012844632,0.00002251147,0.0000335771,0.000022459191,0.98956645,0.00093708216,0.002655285,0.000094585135,0.0057894825],"study_design_scores_gemma":[7.663047e-7,0.000001420235,0.00003769667,4.2686844e-7,7.00168e-7,0.0000011733549,5.411408e-7,0.99944717,0.00008127128,0.00042026973,0.0000078234225,7.757466e-7],"about_ca_topic_score_codex":0.012754995,"about_ca_topic_score_gemma":0.008723128,"teacher_disagreement_score":0.012754995,"about_ca_system_score_codex":0.0011396946,"about_ca_system_score_gemma":0.0006131851,"threshold_uncertainty_score":0.025361538},"labels":[],"label_agreement":null},{"id":"W4382933463","doi":"10.3847/1538-4357/acd2c8","title":"Rotation in Event Horizon Telescope Movies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Oak Ridge National Laboratory; U.S. Department of Energy; Argonne National Laboratory; Institut Périmètre de physique théorique; Natural Sciences and Engineering Research Council of Canada; Office of International Science and Engineering; Office of Science; University of Illinois at Urbana-Champaign; National Science Foundation; Government of Canada; Ministero dello Sviluppo Economico; Innovation, Science and Economic Development Canada","keywords":"Physics; Astrophysics; Rotation (mathematics); Sagittarius A*; Supermassive black hole; Event horizon; Black hole (networking); Astronomy; Telescope; Event (particle physics); Galaxy; Geometry","score_opus":0.014498788978384006,"score_gpt":0.254123105899719,"score_spread":0.23962431692133498,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382933463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9376432,0.00017744262,0.04086645,0.0002398972,0.00009770775,0.00007525197,0.009505663,0.0019569686,0.00943742],"genre_scores_gemma":[0.97803986,0.00005840381,0.016514678,0.000024533958,0.000024605963,0.000011818823,0.003928596,0.00013632634,0.0012611272],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998933,0.00001538313,0.000005218451,0.000031996595,0.000035993642,0.000018116336],"domain_scores_gemma":[0.9993154,0.00017516696,0.00013276174,0.00013501947,0.00016009602,0.000081579776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024860265,0.00015258986,0.000118769174,0.0005818537,0.00018118836,0.00042904666,0.00020456189,0.00020281071,0.0030095463],"category_scores_gemma":[0.001564426,0.00016001808,0.00020059253,0.00059343857,0.00014241692,0.00030057822,0.00019071586,0.0002444947,0.00041760452],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023835697,0.00032411967,0.22510228,0.00048940844,0.00038217774,0.0012811618,0.0010874198,0.18545821,0.30301568,0.01850257,0.032919087,0.22905427],"study_design_scores_gemma":[0.00008504027,0.00027206528,0.3896431,0.00005218838,0.000049211474,0.0006680042,0.00021833203,0.53859204,0.047156878,0.004479289,0.01871288,0.00007096333],"about_ca_topic_score_codex":0.004397033,"about_ca_topic_score_gemma":0.0044042007,"teacher_disagreement_score":0.004397033,"about_ca_system_score_codex":0.00035614904,"about_ca_system_score_gemma":0.00014855023,"threshold_uncertainty_score":0.010067999},"labels":[],"label_agreement":null},{"id":"W4382989179","doi":"10.3847/1538-4357/acd3f0","title":"Inferences from Surface Brightness Fluctuations of Zwicky 3146 via the Sunyaev–Zel’dovich Effect and X-Ray Observations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Nuclear Safety and Security Commission; National Aeronautics and Space Administration","keywords":"Physics; Surface brightness; Astrophysics; X-ray; X-ray background; Astronomy; Brightness; Galaxy; Optics; Active galactic nucleus","score_opus":0.017130274995958313,"score_gpt":0.2409890506584578,"score_spread":0.22385877566249948,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4382989179","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993099,0.000012915198,0.00009074441,0.000009580065,9.937963e-7,0.0000020882076,0.000106954976,0.000005660708,0.00046108148],"genre_scores_gemma":[0.9996425,0.000007334833,0.000055409142,0.0000025087468,0.0000013839759,0.0000016699925,0.00016738511,0.000004054919,0.00011763173],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999198,0.000005365202,0.0000044431777,0.000020603751,0.000025884801,0.000023948114],"domain_scores_gemma":[0.9997004,0.000032721924,0.00012204077,0.000027448505,0.000034930035,0.00008251339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013609836,0.00017925104,0.00024346137,0.0009439726,0.00046032455,0.0004576275,0.00024803515,0.00012669704,0.0012780617],"category_scores_gemma":[0.0006868656,0.00015774672,0.00014550112,0.0006124031,0.0004729164,0.00023994844,0.0007939504,0.00015410336,0.00020525372],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001614332,0.000016857186,0.9685759,0.000012966556,0.00003042891,0.000121746634,0.0003634725,0.0012612487,0.025814267,0.0005116085,0.00029218566,0.0028378612],"study_design_scores_gemma":[0.000001745088,0.000004954188,0.9988273,8.7795405e-7,0.0000013406557,0.000012196098,0.000040595467,0.0005220208,0.000442945,0.00003159095,0.00011316876,0.0000013723503],"about_ca_topic_score_codex":0.017633442,"about_ca_topic_score_gemma":0.0214572,"teacher_disagreement_score":0.017633442,"about_ca_system_score_codex":0.0006925823,"about_ca_system_score_gemma":0.00015312462,"threshold_uncertainty_score":0.035061598},"labels":[],"label_agreement":null},{"id":"W4383047557","doi":"10.3847/1538-4357/ace327","title":"Multiwavelength Observations of the Blazar PKS 0735+178 in Spatial and Temporal Coincidence with an Astrophysical Neutrino Candidate IceCube-211208A","year":2023,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Japan Society for the Promotion of Science; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Science; Australian Research Council; Space Telescope Science Institute; National Commission on Research, Science and Technology; Centre National de la Recherche Scientifique; University of Leicester; Max-Planck-Gesellschaft; National Research Foundation; Austrian Science Fund; Bundesministerium für Bildung und Forschung; Bundesministerium für Bildung, Wissenschaft und Forschung; Irish Research Council; Knut och Alice Wallenbergs Stiftelse; Nuclear Safety and Security Commission; Universiteit van Amsterdam; Deutsche Forschungsgemeinschaft; University of Namibia; EGI Federation; National Science Foundation; Science Foundation Ireland; National Energy Research Scientific Computing Center; U.S. Department of Energy; Smithsonian Institution; Alexander von Humboldt-Stiftung; National Aeronautics and Space Administration","keywords":"Physics; Blazar; Fermi Gamma-ray Space Telescope; Astrophysics; Neutrino; Spectral energy distribution; Photon; Hadron; Gamma ray; Astronomy; Nuclear physics; Galaxy","score_opus":0.023138160033644713,"score_gpt":0.2456019421823805,"score_spread":0.22246378214873577,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383047557","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971222,0.00004993773,0.00014909336,0.000035530193,0.0000051234597,0.000008455877,0.00053083745,0.000029426057,0.0020692851],"genre_scores_gemma":[0.99666303,0.000044948738,0.0011113987,0.000037076366,0.000014738525,0.000014665377,0.0016474362,0.0000111052195,0.00045568688],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999089,0.000009393608,0.0000034864279,0.00002404101,0.00003266713,0.000021498616],"domain_scores_gemma":[0.99974436,0.000026071926,0.00009185531,0.000031138017,0.000037004647,0.00006954218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021176055,0.00023834687,0.00023759858,0.0006880052,0.00047059532,0.0003794607,0.00024812005,0.00024247105,0.00088703464],"category_scores_gemma":[0.0002596888,0.00013374253,0.0002066251,0.0005222363,0.00018112047,0.00017802246,0.00038480677,0.00027369324,0.0002457436],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009589069,0.00028478532,0.8558982,0.000060703023,0.00018125307,0.0017740938,0.0004172601,0.0015281449,0.12181313,0.0005620203,0.0027783194,0.013743098],"study_design_scores_gemma":[0.000036435802,0.00013696232,0.99141836,0.000007920842,0.000030419802,0.00054786383,0.000119871715,0.0013175431,0.003118794,0.000102378115,0.003153584,0.000009940306],"about_ca_topic_score_codex":0.007700761,"about_ca_topic_score_gemma":0.029462926,"teacher_disagreement_score":0.007700761,"about_ca_system_score_codex":0.0005408128,"about_ca_system_score_gemma":0.00024231785,"threshold_uncertainty_score":0.015311897},"labels":[],"label_agreement":null},{"id":"W4383066621","doi":"10.3847/1538-4357/acd44d","title":"Cosmological Information in the Marked Power Spectrum of the Galaxy Field","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Science and Technology Facilities Council","keywords":"Physics; Galaxy; Astrophysics; Spectral density; Redshift; Spectral line; Field (mathematics); Statistics; Astronomy","score_opus":0.0065718067696999,"score_gpt":0.2075529816069068,"score_spread":0.2009811748372069,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383066621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9323912,0.000056861332,0.06292227,0.00017224332,0.000012614593,0.0000123648615,0.0004299532,0.00013131152,0.0038712507],"genre_scores_gemma":[0.9957066,0.000017593577,0.0038000348,0.000020736605,0.000007763031,0.000004319475,0.00019961788,0.000017658795,0.00022574326],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99960226,0.00016406053,0.000018180406,0.00008700194,0.00009196716,0.000036476034],"domain_scores_gemma":[0.993228,0.004231488,0.0006781699,0.0011477333,0.0004964553,0.00021806016],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015408773,0.00027138714,0.00024483385,0.00097560557,0.0002198255,0.000853891,0.00037235947,0.00025509688,0.0025353765],"category_scores_gemma":[0.012644716,0.0002193448,0.000298766,0.0005193303,0.0010064945,0.0017404353,0.0006279399,0.0003724605,0.00015698042],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008474129,0.00013656844,0.2079165,0.00017628989,0.00035121274,0.0005457681,0.00039097283,0.48641425,0.037002753,0.19045952,0.0033731586,0.072385564],"study_design_scores_gemma":[0.00005846674,0.00017071134,0.19168183,0.000043537842,0.00006652006,0.00022643807,0.000118840464,0.68539554,0.009833678,0.1104598,0.0018456001,0.00009909966],"about_ca_topic_score_codex":0.0015544433,"about_ca_topic_score_gemma":0.0017310889,"teacher_disagreement_score":0.0025353765,"about_ca_system_score_codex":0.000426481,"about_ca_system_score_gemma":0.00021953393,"threshold_uncertainty_score":0.008481681},"labels":[],"label_agreement":null},{"id":"W4383101590","doi":"10.3847/1538-4357/acd188","title":"Revealing the Dynamic Magnetoionic Environments of Repeating Fast Radio Burst Sources through Multiyear Polarimetric Monitoring with CHIME/FRB","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; University of Toronto; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Research Chairs; National Defense Science and Engineering Graduate; U.S. Department of Defense; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Physics; Pulsar; Astrophysics; Fast radio burst; Line-of-sight; Milky Way; Polarimetry; Polarization (electrochemistry); Galaxy; Population; Linear polarization; Astronomy; Scattering; Optics","score_opus":0.01188998258854643,"score_gpt":0.2933814059059216,"score_spread":0.28149142331737514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383101590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948901,0.00017056316,0.0010587565,0.000060691942,0.000006932847,0.00001445161,0.0017599983,0.000058344835,0.001980104],"genre_scores_gemma":[0.9960257,0.00010684387,0.0016794256,0.000035505236,0.0000106508605,0.000010387904,0.0016625029,0.000017003074,0.0004518503],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998661,0.000007003256,0.0000034620723,0.000033747678,0.000043794902,0.000045911547],"domain_scores_gemma":[0.99952364,0.000027273354,0.00015632022,0.00005146185,0.000118047465,0.00012327163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030785194,0.00018956642,0.00020714033,0.001573578,0.0005857512,0.00055147137,0.0003004052,0.00019258396,0.00091546203],"category_scores_gemma":[0.0004326418,0.00017091482,0.00014473825,0.0012574752,0.0002914395,0.00023798808,0.0006009927,0.00030628455,0.0002135395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012807758,0.000034030974,0.9001937,0.000031700278,0.00010033979,0.00017715461,0.0004789135,0.00050210464,0.07958578,0.00019498532,0.0009994932,0.017573684],"study_design_scores_gemma":[0.0000021007531,0.00000569639,0.99840575,0.0000019858674,0.0000079505635,0.000052545885,0.00006383217,0.00020574371,0.00066821673,0.000017436174,0.00056363916,0.00000506745],"about_ca_topic_score_codex":0.09529153,"about_ca_topic_score_gemma":0.23891899,"teacher_disagreement_score":0.09529153,"about_ca_system_score_codex":0.0006436678,"about_ca_system_score_gemma":0.0004403111,"threshold_uncertainty_score":0.18947375},"labels":[],"label_agreement":null},{"id":"W4383102408","doi":"10.3847/1538-4357/acd333","title":"All-sky Faint DA White Dwarf Spectrophotometric Standards for Astrophysical Observatories: The Complete Sample","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Los Alamos National Laboratory; Argonne National Laboratory; High Energy Physics; Division of Astronomical Sciences; Leibniz-Gemeinschaft; Science Mission Directorate; University of North Carolina at Chapel Hill; College of Engineering, Michigan State University; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; University of Colorado Boulder; Office of Science; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astrophysik; Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Eötvös Loránd Tudományegyetem; Yale University; U.S. Department of Energy; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Science and Technology Facilities Council; York University; Ministério da Ciência, Tecnologia e Inovação; Integrated Electronics Engineering Center, Binghamton University; University of Edinburgh; Queen's University; Chinese Academy of Sciences; Deutsche Forschungsgemeinschaft; National Central University; Institut de Física d'Altes Energies; Space Telescope Science Institute; University of Sussex; University of Nottingham; European Commission; University of Oxford; University of Cambridge; Durham University; University of Chicago; National Energy Research Scientific Computing Center; Instituto de Astrofísica de Canarias; Carnegie Institution for Science; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; National Science Foundation; University of Michigan; University of Notre Dame; Smithsonian Astrophysical Observatory; European Space Agency; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Planetary Science Division; Carnegie Institution of Washington; University of Portsmouth; New Mexico State University; University of Utah; Carnegie Mellon University; Fermilab; Max-Planck-Institut für Astronomie; Michigan State University; Vanderbilt University; Ohio State University; Smithsonian Institution; Financiadora de Estudos e Projetos; University of Pennsylvania; University College London; National Aeronautics and Space Administration; Queen's University Belfast; Gordon and Betty Moore Foundation; California Institute of Technology","keywords":"Physics; White dwarf; Sky; Astrophysics; Astronomy; Sample (material); Stars","score_opus":0.03867652231483143,"score_gpt":0.28092424902122337,"score_spread":0.24224772670639194,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383102408","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8915496,0.00072926725,0.003930447,0.00012688026,0.00003765163,0.00014070762,0.08841718,0.000498703,0.014569497],"genre_scores_gemma":[0.7915534,0.00044662514,0.005663354,0.00012316818,0.000091466856,0.00024381252,0.19063659,0.0002826859,0.010958958],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99905807,0.000074527146,0.00010712665,0.0002515817,0.0003639266,0.00014483236],"domain_scores_gemma":[0.9970765,0.00017975329,0.0005477945,0.0007789585,0.0009216631,0.0004952809],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000773988,0.00044685087,0.00043173396,0.002581469,0.00040223167,0.0007320093,0.00055380014,0.00020977926,0.0050352295],"category_scores_gemma":[0.001764642,0.00018718585,0.00033255987,0.0025718794,0.00018077057,0.0004973768,0.0010876086,0.00028245384,0.004952364],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030881565,0.00015045896,0.908749,0.00012181086,0.000097050535,0.000099854136,0.00038485872,0.00035999034,0.009253649,0.00097522786,0.021126859,0.058372498],"study_design_scores_gemma":[0.000016079232,0.00004362044,0.96115696,0.00001243174,0.00002698227,0.00010516551,0.00018983484,0.00038433145,0.001580337,0.00014177895,0.036336545,0.0000059749705],"about_ca_topic_score_codex":0.0076100784,"about_ca_topic_score_gemma":0.007035724,"teacher_disagreement_score":0.0076100784,"about_ca_system_score_codex":0.00033143247,"about_ca_system_score_gemma":0.0007604253,"threshold_uncertainty_score":0.016844511},"labels":[],"label_agreement":null},{"id":"W4383102441","doi":"10.3847/1538-4357/acd336","title":"The Next Generation Virgo Cluster Survey (NGVS). XXXV. First Kinematical Clues of Overly Massive Dark Matter Halos in Several Ultradiffuse Galaxies in the Virgo Cluster","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Virgo Cluster; Astrophysics; Velocity dispersion; Galaxy; Dark matter; Astronomy; Dark galaxy; Milky Way; Dwarf spheroidal galaxy; Dwarf galaxy; Galaxy cluster; Luminosity; Globular cluster; Brightest cluster galaxy; Galaxy group","score_opus":0.020820767573485784,"score_gpt":0.23421143087178628,"score_spread":0.2133906632983005,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383102441","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98510796,0.0005801916,0.000390008,0.00017131174,0.000013482372,0.000021982067,0.009645628,0.000084073865,0.003985359],"genre_scores_gemma":[0.9840443,0.000152892,0.0007769904,0.00009460482,0.00001032955,0.000015339037,0.0132419,0.000016416414,0.0016470831],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989855,0.000014523807,0.000003908478,0.00002290859,0.000023417524,0.000036714355],"domain_scores_gemma":[0.9997385,0.000021365584,0.00004526805,0.00004509264,0.000035083205,0.000114750714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026668425,0.00014313684,0.00013397266,0.001560086,0.00030242308,0.00040089418,0.00021354521,0.00020101662,0.0017947688],"category_scores_gemma":[0.00041903212,0.00007819808,0.00017664961,0.00077829405,0.00012631596,0.00014958587,0.00055834954,0.0001723392,0.00045790305],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008710915,0.000024009794,0.9796198,0.000025898264,0.000057819005,0.00011365325,0.00013513748,0.0003286598,0.0034166137,0.0004311239,0.0037714397,0.011988709],"study_design_scores_gemma":[0.0000023874136,0.000009220875,0.99558973,0.000006397598,0.0000090799,0.000054808388,0.00006960836,0.00023923596,0.0003406676,0.00009412982,0.0035814948,0.0000031606774],"about_ca_topic_score_codex":0.017917126,"about_ca_topic_score_gemma":0.036239218,"teacher_disagreement_score":0.017917126,"about_ca_system_score_codex":0.0004636923,"about_ca_system_score_gemma":0.00017362127,"threshold_uncertainty_score":0.035625696},"labels":[],"label_agreement":null},{"id":"W4383217426","doi":"10.3847/1538-4357/acd2ca","title":"Constraints on Populations of Neutrino Sources from Searches in the Directions of IceCube Neutrino Alerts","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Alberta","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; National Research Foundation; Michigan State University; University of Oxford; Chiba University; Santen; Compute Canada; Marquette University","keywords":"Physics; Neutrino; Neutrino astronomy; Neutrino detector; Astronomy; Solar neutrino problem; Particle physics; Astrophysics; Neutrino oscillation; Solar neutrino","score_opus":0.03435234167909117,"score_gpt":0.26960783771256586,"score_spread":0.23525549603347468,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383217426","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9900967,0.00031415996,0.0030374038,0.000059658007,0.000014768885,0.000023524211,0.0021565754,0.000050294606,0.0042469194],"genre_scores_gemma":[0.9918019,0.00019546533,0.0022135153,0.000036805,0.00003148843,0.000025298312,0.005349851,0.000029977093,0.00031567886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991825,0.00018431642,0.00007073071,0.00026093892,0.00016765484,0.00013369096],"domain_scores_gemma":[0.99406046,0.002794607,0.001790815,0.00048374193,0.00046280344,0.00040759266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015579179,0.00043153073,0.0004544883,0.0020991596,0.0004892085,0.0017462266,0.00047027334,0.00044274912,0.0021102058],"category_scores_gemma":[0.0059351358,0.00041916434,0.00054788095,0.0009764355,0.00033209258,0.00073790486,0.00093317946,0.00030831574,0.00040232448],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005259813,0.000051567535,0.9732564,0.00004602566,0.00017778394,0.00012337315,0.00016507921,0.002218003,0.010714976,0.0015205323,0.0006885245,0.010511834],"study_design_scores_gemma":[0.000035442565,0.000079932775,0.96645474,0.00005820243,0.0001417831,0.00051046716,0.00029277173,0.018064482,0.008417488,0.0018886933,0.0040288707,0.000027054257],"about_ca_topic_score_codex":0.003030813,"about_ca_topic_score_gemma":0.0039076214,"teacher_disagreement_score":0.003030813,"about_ca_system_score_codex":0.00040836242,"about_ca_system_score_gemma":0.00031134608,"threshold_uncertainty_score":0.00823915},"labels":[],"label_agreement":null},{"id":"W4383225811","doi":"10.3847/1538-4357/acd936","title":"The Evolution of Population III and Extremely Metal-poor Binary Stars","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Office of Science; National Science and Technology Council; National Energy Research Scientific Computing Center; Academia Sinica; U.S. Department of Energy","keywords":"Physics; Stars; Astrophysics; Binary number; Binary star; Astronomy; Stellar evolution; Population; Demography; Sociology","score_opus":0.014040368062450645,"score_gpt":0.23169216822818448,"score_spread":0.21765180016573382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383225811","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979255,0.00003074247,0.00045902966,0.000031928663,0.000002300686,0.0000026004484,0.00010683757,0.000017576705,0.0014234567],"genre_scores_gemma":[0.99924743,0.000017056607,0.0003384274,0.000013333795,0.0000012363898,0.0000035491619,0.00012351443,0.000013213222,0.00024229441],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999292,0.00001733022,0.0000042455354,0.000016296002,0.0000130101225,0.000019888343],"domain_scores_gemma":[0.9995129,0.00016178684,0.00010299099,0.000036886657,0.00004809423,0.00013734365],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003117753,0.00023554444,0.00029050102,0.00047450425,0.0005580824,0.0008235972,0.00044079364,0.00041065572,0.0011297],"category_scores_gemma":[0.0012174092,0.00021182356,0.00029464543,0.0005527154,0.00039826072,0.0003340728,0.0007623941,0.00038648967,0.00018684722],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048288156,0.00018194776,0.43425515,0.00006267142,0.00025899406,0.000747499,0.00042369304,0.50477976,0.033868797,0.016410643,0.0011744741,0.0073534898],"study_design_scores_gemma":[0.000106440486,0.000114769995,0.17186257,0.000020451605,0.00006151567,0.00029338727,0.0003285191,0.81120676,0.010303215,0.0037620638,0.0019039664,0.00003627404],"about_ca_topic_score_codex":0.0064932387,"about_ca_topic_score_gemma":0.0043241563,"teacher_disagreement_score":0.0064932387,"about_ca_system_score_codex":0.000773585,"about_ca_system_score_gemma":0.0003256435,"threshold_uncertainty_score":0.0129109025},"labels":[],"label_agreement":null},{"id":"W4383265835","doi":"10.3847/1538-4357/acd4c5","title":"From Dust to Nanodust: Resolving Circumstellar Dust from the Colliding-wind Binary Wolf-Rayet 140","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Institutes of Natural Sciences; Japan Society for the Promotion of Science; National Aeronautics and Space Administration; California Institute of Technology; Japan Aerospace Exploration Agency; W. M. Keck Foundation; Deutsche Forschungsgemeinschaft; National Science Foundation","keywords":"Physics; Astrophysics; Circumstellar dust; Astronomy; Cosmic dust; Interplanetary dust cloud; Infrared; Radiative transfer; Infrared excess; Spectral energy distribution; Solar System; Galaxy","score_opus":0.018505739659388582,"score_gpt":0.24627242276566338,"score_spread":0.2277666831062748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383265835","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99810225,0.00015513225,0.000480639,0.00002128875,0.0000072403564,0.000006150697,0.0003000731,0.00004043055,0.00088680885],"genre_scores_gemma":[0.9969031,0.00007313501,0.0018804062,0.000034363446,0.000017064564,0.000005137245,0.0006808328,0.000016585096,0.00038931533],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99994683,0.0000019955007,0.0000025222919,0.00002036764,0.000013999143,0.000014343003],"domain_scores_gemma":[0.9999279,0.0000063751677,0.00001703102,0.000006207055,0.000014809188,0.000027754413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007001297,0.00014947893,0.00017855149,0.0008412784,0.00027988682,0.00032940792,0.00024357795,0.0002301481,0.000829025],"category_scores_gemma":[0.000089522124,0.000121875906,0.00014512826,0.000359461,0.00008818015,0.00024840696,0.00030768174,0.00018961054,0.00026246093],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033128582,0.00018249797,0.3814551,0.00007718185,0.00008819691,0.0020472242,0.0003269856,0.000622327,0.5901733,0.00013897756,0.0010628777,0.023493992],"study_design_scores_gemma":[0.000012688423,0.000106217594,0.9639714,0.000011666827,0.000033079297,0.0014160597,0.00057726767,0.0038759669,0.027383713,0.00015500562,0.0024465253,0.000010446971],"about_ca_topic_score_codex":0.0010917188,"about_ca_topic_score_gemma":0.0038003398,"teacher_disagreement_score":0.0010917188,"about_ca_system_score_codex":0.000118436,"about_ca_system_score_gemma":0.00007273293,"threshold_uncertainty_score":0.0027733445},"labels":[],"label_agreement":null},{"id":"W4383295340","doi":"10.3847/1538-4357/acd4bd","title":"Stellar Characterization and Radius Inflation of Hyades M-dwarf Stars from the APOGEE Survey","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Science Mission Directorate; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Astrophysics Division; York University; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Banco Santander; Leibniz-Gemeinschaft; University of Notre Dame; U.S. Department of Energy; Smithsonian Institution; Ministério da Ciência, Tecnologia e Inovação; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; National Aeronautics and Space Administration; Max-Planck-Institut für Astrophysik; National Science Foundation","keywords":"Physics; Astrophysics; Stars; RADIUS; Metallicity; Open cluster; Effective temperature; Spectral line; Astronomy; Stellar evolution","score_opus":0.018058099702950723,"score_gpt":0.2263298007475856,"score_spread":0.20827170104463488,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383295340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999624,0.00002383221,0.00004215737,0.0000040292866,3.7862455e-7,9.079596e-7,0.00017946819,0.0000034182417,0.00012173759],"genre_scores_gemma":[0.9990476,0.000021136453,0.000095905794,0.000004584088,0.0000018934916,0.000002099371,0.00069970626,0.0000028892212,0.00012426825],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998672,0.00002173933,0.000012082831,0.000045172055,0.000030263145,0.00002352416],"domain_scores_gemma":[0.9994191,0.00007093026,0.00021116897,0.00009529203,0.00008937893,0.00011427707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002866209,0.00016188443,0.00019628556,0.0010875133,0.0002240027,0.0003551768,0.00014854102,0.00014722005,0.00058457855],"category_scores_gemma":[0.0006869026,0.00009275115,0.00016077238,0.0005574397,0.00018658675,0.00022383661,0.00042591218,0.00010827534,0.00027577323],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000056449797,0.000007943349,0.9957396,0.000003936254,0.000011933117,0.000021175762,0.00013476427,0.00009215629,0.0022348322,0.000030298908,0.00007217368,0.0015948453],"study_design_scores_gemma":[5.588993e-7,0.000007967227,0.99962854,4.290185e-7,0.000001937368,0.000023630173,0.000041057814,0.000082175124,0.00012818184,0.000005792082,0.00007905795,6.26708e-7],"about_ca_topic_score_codex":0.0040254425,"about_ca_topic_score_gemma":0.0055216216,"teacher_disagreement_score":0.0040254425,"about_ca_system_score_codex":0.00022391175,"about_ca_system_score_gemma":0.00008769998,"threshold_uncertainty_score":0.00800401},"labels":[],"label_agreement":null},{"id":"W4383343713","doi":"10.3847/1538-4357/accd5d","title":"Mapping the Skies of Ultracool Worlds: Detecting Storms and Spots with Extremely Large Telescopes","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Science Foundation","keywords":"Physics; Exoplanet; Starspot; Brown dwarf; Astronomy; Stars; Astrophysics; Spectrograph; Spectral line","score_opus":0.015604710652360297,"score_gpt":0.21795324145215103,"score_spread":0.20234853079979073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383343713","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9407053,0.00022193063,0.03876618,0.00016044383,0.000036254823,0.00010470951,0.0036734384,0.012093064,0.004238742],"genre_scores_gemma":[0.913329,0.000049336035,0.08103575,0.000048182595,0.000014158972,0.00004134905,0.0044954787,0.0005057428,0.0004810541],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995165,0.000088450186,0.00002232031,0.00013101759,0.00016140263,0.00008028766],"domain_scores_gemma":[0.9994178,0.00018438093,0.00010113431,0.00010706358,0.00009657779,0.00009297331],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008809612,0.00036496512,0.0002865526,0.0008232013,0.00025297204,0.00060533534,0.0008859391,0.00033157214,0.0012938405],"category_scores_gemma":[0.0020536107,0.0002725285,0.00038718313,0.0010116001,0.0003104974,0.00076442125,0.0010162367,0.0003523773,0.00057105353],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013272961,0.00057779235,0.36646986,0.0003273351,0.0005856517,0.000663165,0.0011299594,0.32183552,0.05873,0.0033109335,0.025129696,0.21991283],"study_design_scores_gemma":[0.00014044918,0.00014214298,0.113553,0.00002510016,0.000044837074,0.0001135202,0.00022214034,0.8670899,0.012884293,0.0015331566,0.0042050118,0.000046428835],"about_ca_topic_score_codex":0.012212613,"about_ca_topic_score_gemma":0.015496808,"teacher_disagreement_score":0.012212613,"about_ca_system_score_codex":0.0004549478,"about_ca_system_score_gemma":0.0004062653,"threshold_uncertainty_score":0.024283051},"labels":[],"label_agreement":null},{"id":"W4383369950","doi":"10.3847/1538-4357/acd16f","title":"The Hazy and Metal-rich Atmosphere of GJ 1214 b Constrained by Near- and Mid-infrared Transmission Spectroscopy","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":72,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Haze; Physics; Atmosphere (unit); Exoplanet; Infrared; Spectroscopy; Astrophysics; Metallicity; Atmospheric sciences; Astronomy; Stars; Meteorology","score_opus":0.006364018362578749,"score_gpt":0.20878597650928818,"score_spread":0.20242195814670944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383369950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987244,0.000035708956,0.00022944635,0.000033521606,0.0000021554138,0.000005955257,0.00041385743,0.000085963395,0.0004690111],"genre_scores_gemma":[0.99865925,0.000019650271,0.00032527273,0.000014860071,0.0000036773997,0.0000046636774,0.0008823976,0.000020251216,0.00006999518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998889,0.000020341498,0.000005186204,0.000034356563,0.000019976234,0.00003111598],"domain_scores_gemma":[0.9997743,0.000041087147,0.000038948194,0.0000358721,0.000021182088,0.000088600165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028835755,0.0006677417,0.000341574,0.0006387685,0.00047523173,0.000549465,0.0004957046,0.00071346655,0.0010172892],"category_scores_gemma":[0.0005010995,0.00034847498,0.00071253633,0.0005158896,0.00034468048,0.0003279743,0.0006828022,0.00030413535,0.0002561969],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010126156,0.0004116163,0.6755425,0.00018268732,0.00061533035,0.0014372529,0.0005191226,0.18445815,0.123345844,0.0014237524,0.0020220373,0.009029158],"study_design_scores_gemma":[0.0002470774,0.00020885764,0.8104414,0.000016213955,0.00013027838,0.00012208447,0.00025798444,0.1830735,0.0038381675,0.00042480972,0.0011878154,0.00005183411],"about_ca_topic_score_codex":0.028667476,"about_ca_topic_score_gemma":0.017047834,"teacher_disagreement_score":0.028667476,"about_ca_system_score_codex":0.0005460011,"about_ca_system_score_gemma":0.00026634656,"threshold_uncertainty_score":0.057001233},"labels":[],"label_agreement":null},{"id":"W4383375295","doi":"10.3847/1538-4357/accc2a","title":"Multiphase Gas Interactions on Subarcsec Scales in the Shocked Intergalactic Medium of Stephan’s Quintet with JWST and ALMA","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Astronomical Observatory of Japan; Institut Universitaire de France; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Sorbonne Université; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; James Webb Space Telescope; Galaxy; Interstellar medium; Spitzer Space Telescope; Intergalactic travel; Astronomy; Molecular cloud; Telescope; Stars","score_opus":0.01062802612993143,"score_gpt":0.2438028983658791,"score_spread":0.23317487223594766,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383375295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994993,0.0000130881635,0.000040654682,0.000017461047,0.0000010245442,0.0000014384553,0.000032851713,0.0000059235786,0.00038822688],"genre_scores_gemma":[0.9997435,0.0000057413736,0.00007144639,0.000006796841,0.0000011137403,0.000001006476,0.000052888812,0.0000016235127,0.00011590735],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999416,0.000003609829,0.0000010186322,0.000017360308,0.000015215641,0.000021132802],"domain_scores_gemma":[0.9998809,0.0000109496605,0.000029843279,0.000009374078,0.000018509096,0.00005047769],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000059041762,0.00012864853,0.000120226556,0.00047688643,0.00043957488,0.00035138417,0.00033935872,0.00013899192,0.0012744956],"category_scores_gemma":[0.00016567584,0.000099545694,0.00011317781,0.00033272099,0.00027650248,0.00028971967,0.00063244725,0.00021724305,0.00009458574],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047954684,0.00016970462,0.82732534,0.00003472779,0.00013924555,0.0062764706,0.0019928396,0.0021411336,0.14522344,0.0008779878,0.0008985854,0.014441074],"study_design_scores_gemma":[0.0000084275225,0.000033650704,0.99444515,0.0000020786008,0.00000962491,0.0002687799,0.0004533129,0.002213623,0.0016712344,0.000112922266,0.00077548,0.000005662484],"about_ca_topic_score_codex":0.016738031,"about_ca_topic_score_gemma":0.023068974,"teacher_disagreement_score":0.016738031,"about_ca_system_score_codex":0.00040982934,"about_ca_system_score_gemma":0.00015188451,"threshold_uncertainty_score":0.033281207},"labels":[],"label_agreement":null},{"id":"W4383557318","doi":"10.3847/1538-4357/acd4be","title":"CLEAR: The Morphological Evolution of Galaxies in the Green Valley","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Galaxy; Astrophysics; Astronomy; Galaxy formation and evolution","score_opus":0.013192290663255038,"score_gpt":0.22548147827464315,"score_spread":0.21228918761138812,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383557318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99121314,0.000072819115,0.0013766137,0.00024079275,0.0000056225326,0.000006279564,0.0012964826,0.000115525356,0.0056727137],"genre_scores_gemma":[0.99626774,0.000025882438,0.00070233387,0.000038558246,0.0000024710282,0.0000040866444,0.0008319794,0.000047709895,0.002079177],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999255,0.000014927024,0.0000016175225,0.000023471906,0.000014295817,0.000020118272],"domain_scores_gemma":[0.9997373,0.000059879145,0.000037696107,0.00003725683,0.00003381462,0.00009401841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002041062,0.00012440661,0.0001575118,0.00034659047,0.00030274616,0.0012288913,0.0005589137,0.00038278202,0.005138251],"category_scores_gemma":[0.0008680976,0.00015126215,0.00028524286,0.00047809328,0.00045664876,0.0007873545,0.0007394415,0.0003817016,0.0006887311],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008116913,0.0002999019,0.6629835,0.00009470335,0.00013334645,0.0010134343,0.003039029,0.23757517,0.008433571,0.040604204,0.013884725,0.031126695],"study_design_scores_gemma":[0.00016422266,0.00016883737,0.5882227,0.000038908107,0.00003122439,0.0002493932,0.0016813496,0.3668081,0.00096796936,0.02497878,0.016633013,0.00005554243],"about_ca_topic_score_codex":0.04019625,"about_ca_topic_score_gemma":0.044238478,"teacher_disagreement_score":0.04019625,"about_ca_system_score_codex":0.0006090234,"about_ca_system_score_gemma":0.00032119852,"threshold_uncertainty_score":0.079924524},"labels":[],"label_agreement":null},{"id":"W4383557692","doi":"10.3847/1538-4357/acd340","title":"Mapping the Multiphase Structure of H i in the Low-latitude Intermediate-velocity Arch 1","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Astrophysics Division; Natural Sciences and Engineering Research Council of Canada; University of Toronto; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Absorption (acoustics); Turbulence; Spectral line; Spectral resolution; Optics; Thermodynamics; Astronomy","score_opus":0.01503586940552602,"score_gpt":0.24722671151521672,"score_spread":0.2321908421096907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383557692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987563,0.00004073001,0.0002362452,0.000009705414,0.0000016365896,0.0000033824651,0.00020575942,0.00003084195,0.00071540993],"genre_scores_gemma":[0.9988972,0.000017264914,0.00035196618,0.000006297727,0.0000024416945,0.0000026054938,0.00052677374,0.000013852205,0.00018152577],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999944,0.0000035574697,0.0000014647453,0.000018705181,0.000010720543,0.000021658592],"domain_scores_gemma":[0.9998323,0.000017425951,0.00004220486,0.000014360604,0.000032830205,0.000060978196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011717013,0.00023044871,0.00018260638,0.00069939945,0.00032668578,0.00058585283,0.00038397478,0.00017109941,0.0010994467],"category_scores_gemma":[0.00025026427,0.00019685927,0.00014870995,0.0004782193,0.00019307909,0.00020601213,0.0004355641,0.00034071246,0.00027383992],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006819692,0.00013880225,0.8516601,0.000060163053,0.000070657494,0.00023679453,0.00063166255,0.005429824,0.1214271,0.00075265206,0.000694482,0.018215848],"study_design_scores_gemma":[0.00001178138,0.000046265755,0.9892335,0.0000067009755,0.000016185515,0.000027343984,0.00013381022,0.006706887,0.0028473241,0.00012497355,0.0008346979,0.000010496459],"about_ca_topic_score_codex":0.012962489,"about_ca_topic_score_gemma":0.019036599,"teacher_disagreement_score":0.012962489,"about_ca_system_score_codex":0.0005495423,"about_ca_system_score_gemma":0.00021086114,"threshold_uncertainty_score":0.025774062},"labels":[],"label_agreement":null},{"id":"W4383875478","doi":"10.3847/1538-4357/acd115","title":"A Novel Survey for Young Substellar Objects with the W-band Filter. VI. Spectroscopic Census of Substellar Members and the IMF of the σ Orionis Cluster","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Université de Montréal","funders":"","keywords":"Brown dwarf; Physics; Astrophysics; Stars; Low Mass; Stellar classification; Astrometry; Astronomy; Cluster (spacecraft); Initial mass function; Pleiades; Open cluster; Star formation","score_opus":0.014423963690156694,"score_gpt":0.236761984931937,"score_spread":0.22233802124178031,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4383875478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932678,0.00017094956,0.0014219241,0.000022470196,0.000004475161,0.000046933226,0.0032219505,0.00009559925,0.0017478942],"genre_scores_gemma":[0.98148626,0.00018456136,0.0047853366,0.00003419526,0.00002974644,0.00006508941,0.01013192,0.000025685622,0.0032572048],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983,0.000015063017,0.00001372003,0.000061316394,0.00004169286,0.00003817999],"domain_scores_gemma":[0.9993635,0.000040462503,0.0001567838,0.000078944184,0.00014833012,0.0002120403],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025633958,0.00020285751,0.00018159117,0.002545219,0.0003837312,0.00038052228,0.0002730682,0.0002030857,0.0024154866],"category_scores_gemma":[0.00036879827,0.00011429032,0.00020085051,0.0015716201,0.000108448214,0.00032857456,0.00044812032,0.00012851245,0.0011575486],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007029902,0.00006834609,0.94092935,0.000038990038,0.000030302548,0.00016775411,0.0003177054,0.000092965485,0.030696632,0.00010495572,0.0008780007,0.02660471],"study_design_scores_gemma":[0.0000030172173,0.00003436383,0.99670804,0.000002680862,0.000009356325,0.00014892829,0.0000718525,0.0002367943,0.0010232772,0.000019960808,0.001739203,0.0000025233558],"about_ca_topic_score_codex":0.0070868325,"about_ca_topic_score_gemma":0.012361147,"teacher_disagreement_score":0.0070868325,"about_ca_system_score_codex":0.0001524197,"about_ca_system_score_gemma":0.00024437814,"threshold_uncertainty_score":0.014091194},"labels":[],"label_agreement":null},{"id":"W4384068374","doi":"10.3847/1538-4357/acd54c","title":"Flares, Warps, Truncations, and Satellite: The Ultra-thin Galaxy UGC 11859","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; York University; Universities Space Research Association; Space Telescope Science Institute; Carnegie Mellon University; Ames Research Center; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; National Aeronautics and Space Administration; Brookhaven National Laboratory; U.S. Department of Energy","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Surface brightness; Satellite galaxy; Photometry (optics); RADIUS; Thin disk; Disc; Galaxy formation and evolution; Stars","score_opus":0.009026334337025547,"score_gpt":0.21835952886364313,"score_spread":0.20933319452661758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384068374","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997855,0.00009008902,0.0002932008,0.000051752282,0.00000342208,0.0000049000614,0.00031871634,0.00003351639,0.0013493611],"genre_scores_gemma":[0.99893135,0.000025735415,0.0003590157,0.000027551283,0.0000029635876,0.000001988183,0.00042024357,0.000011872736,0.00021922072],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991834,0.0000073393335,0.0000041265644,0.000026052998,0.00002181989,0.000022298895],"domain_scores_gemma":[0.99974054,0.00002301195,0.0000699073,0.000041014784,0.00003584165,0.00008962435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011267709,0.00022489403,0.0002305221,0.00066015264,0.00041925485,0.00041929065,0.0003900422,0.00021677602,0.0008183757],"category_scores_gemma":[0.0004362485,0.00018128908,0.0001745345,0.00047672488,0.00043259872,0.00024460125,0.00053914165,0.00034200982,0.00014485948],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007146871,0.00016664415,0.85448277,0.00009229191,0.00022999546,0.0020095268,0.0011760594,0.012096077,0.0873295,0.0032728985,0.003994889,0.03443459],"study_design_scores_gemma":[0.000024024726,0.00004272811,0.98478484,0.000016927948,0.000030959676,0.00025613868,0.0002388042,0.009126707,0.0027806188,0.0005680138,0.0021128552,0.000017429675],"about_ca_topic_score_codex":0.033248503,"about_ca_topic_score_gemma":0.033913467,"teacher_disagreement_score":0.033248503,"about_ca_system_score_codex":0.0008764087,"about_ca_system_score_gemma":0.00016149513,"threshold_uncertainty_score":0.066109955},"labels":[],"label_agreement":null},{"id":"W4384297188","doi":"10.3847/1538-4357/acd6f2","title":"The JCMT BISTRO Survey: Studying the Complex Magnetic Field of L43","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; McMaster University; Queen's University; University of Manitoba; Herzberg Institute of Astrophysics; University of Victoria; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Agencia Estatal de Investigación; Science and Engineering Research Board; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; Agencia Canaria de Investigación, Innovación y Sociedad de la Información; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; European Regional Development Fund; Academia Sinica; National Natural Science Foundation of China; Department of Science and Technology, Ministry of Science and Technology, India; National Key Research and Development Program of China; Science and Technology Facilities Council; National Research Foundation; National Science Foundation; Royal Society; National Astronomical Research Institute of Thailand; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute","keywords":"James Clerk Maxwell Telescope; Protostar; Outflow; Astrophysics; Physics; Ophiuchus; Magnetic field; Protein filament; Molecular cloud; Core (optical fiber); Field (mathematics); Bipolar outflow; Star formation; Telescope; Stars; Chemistry; Optics; Meteorology","score_opus":0.03832150306000825,"score_gpt":0.28844324433701574,"score_spread":0.2501217412770075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384297188","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995374,0.00012546289,0.00036076104,0.00012290699,0.0000058588685,0.000012453479,0.000885865,0.00010200275,0.0030107447],"genre_scores_gemma":[0.99623245,0.00009650815,0.0010360663,0.000121580764,0.0000192468,0.000012191706,0.0017555046,0.000061355255,0.0006651005],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998684,0.000016925636,0.00000382046,0.000025551417,0.000043982644,0.00004129569],"domain_scores_gemma":[0.9996344,0.000020769721,0.00008689363,0.00005788982,0.00005594929,0.00014401817],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025305332,0.00020167799,0.00022782576,0.00068089727,0.00043043582,0.0004350923,0.00027721174,0.00025938245,0.0012566904],"category_scores_gemma":[0.0004237567,0.00014736388,0.00014733296,0.0005952802,0.00017326933,0.0002460003,0.00063498784,0.00032994314,0.00044954722],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042513374,0.0002933136,0.77031034,0.00010106916,0.00019647105,0.0010974512,0.00139744,0.0015670144,0.1736589,0.0010149045,0.0075771236,0.04236083],"study_design_scores_gemma":[0.000021749689,0.00005177972,0.99094254,0.000008038786,0.000015163151,0.00012950628,0.00014884889,0.0015090201,0.0019743906,0.0000736672,0.0051167593,0.000008501792],"about_ca_topic_score_codex":0.013344208,"about_ca_topic_score_gemma":0.029869437,"teacher_disagreement_score":0.013344208,"about_ca_system_score_codex":0.00043867136,"about_ca_system_score_gemma":0.00031062233,"threshold_uncertainty_score":0.026533067},"labels":[],"label_agreement":null},{"id":"W4384699472","doi":"10.3847/1538-4357/acda94","title":"Magnetic Effects Promote Supermassive Star Formation in Metal-enriched Atomic-cooling Halos","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Japan Society for the Promotion of Science","keywords":"Physics; Protostar; Astrophysics; Star formation; Supermassive black hole; Accretion (finance); Magnetic field; Angular momentum; Halo; Structure formation; Stars; Galaxy; Classical mechanics","score_opus":0.009323843102187425,"score_gpt":0.2339462171761481,"score_spread":0.22462237407396068,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384699472","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976859,0.00005154738,0.00038094824,0.00008145429,0.0000075005323,0.00000867933,0.000044389737,0.000035717443,0.0017038019],"genre_scores_gemma":[0.99968123,0.000020972288,0.00013132203,0.000023278406,0.0000032012833,0.0000030096455,0.000022559409,0.000004660634,0.0001097827],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999201,0.000013724461,0.000002600522,0.000007899761,0.000008297563,0.000047299945],"domain_scores_gemma":[0.99970514,0.000056187677,0.000063203275,0.000019234114,0.000025759526,0.00013056779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017107885,0.00036031049,0.00034677936,0.00037871496,0.0006642058,0.00081560726,0.000618261,0.00045144188,0.0017568358],"category_scores_gemma":[0.000742666,0.00024897413,0.0005984454,0.00021895238,0.0006413315,0.00041647366,0.0009229185,0.0003384792,0.00011384013],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008679623,0.0005195194,0.08938786,0.00016442969,0.00037536942,0.0012948565,0.00032170123,0.85259795,0.04204893,0.0074880254,0.0013857696,0.0035476512],"study_design_scores_gemma":[0.0007808869,0.00047634137,0.050788525,0.000023984805,0.00014720188,0.000156878,0.00035715807,0.9378664,0.005785172,0.0024781853,0.0011010164,0.000038232327],"about_ca_topic_score_codex":0.00914845,"about_ca_topic_score_gemma":0.0046798317,"teacher_disagreement_score":0.00914845,"about_ca_system_score_codex":0.0006986064,"about_ca_system_score_gemma":0.00054510956,"threshold_uncertainty_score":0.018190384},"labels":[],"label_agreement":null},{"id":"W4384830712","doi":"10.3847/1538-4357/acd929","title":"The JWST PEARLS View of the El Gordo Galaxy Cluster and of the Structure It Magnifies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Astrophysics Science Division; Division of Graduate Education; Science and Technology Facilities Council; National Science Foundation; NASA Headquarters; Agencia Estatal de Investigación; Goddard Space Flight Center; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Nuclear Safety and Security Commission; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration; United States-Israel Binational Science Foundation","keywords":"Physics; James Webb Space Telescope; Virial mass; Astrophysics; Galaxy; Astronomy; Gravitational lens; Redshift; Reionization; Satellite galaxy; Galaxy cluster; Weak gravitational lensing; Photometry (optics); Galaxy formation and evolution; Stars","score_opus":0.006020886110178825,"score_gpt":0.21429736093677693,"score_spread":0.2082764748265981,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384830712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.73747736,0.003217099,0.004706657,0.009405933,0.00053212955,0.00009813604,0.008650942,0.0024369077,0.23347485],"genre_scores_gemma":[0.92797345,0.00088701944,0.004254716,0.0011846403,0.00061441987,0.000028422462,0.0051719802,0.0005146699,0.059370585],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9999411,0.0000034344346,0.00000144712,0.000013864803,0.000026335048,0.000013758285],"domain_scores_gemma":[0.9998017,0.000011140892,0.000029583176,0.000018879213,0.000031214848,0.000107537235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013394903,0.00023515643,0.00014987013,0.002950145,0.00057968876,0.0012946153,0.00041047353,0.00025699934,0.019336503],"category_scores_gemma":[0.0002378361,0.00013571256,0.00010944846,0.00067575235,0.0003756131,0.0007157428,0.0009884485,0.00042311673,0.0021450417],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035221298,0.00011198928,0.3129793,0.00031048528,0.00012947916,0.0050471984,0.0037022356,0.0020699413,0.054835673,0.021328142,0.40835595,0.19077735],"study_design_scores_gemma":[0.00002866777,0.000049962062,0.6661797,0.000108396554,0.000021204472,0.0016707506,0.0020572613,0.0022816109,0.0027483238,0.00469459,0.32012764,0.00003193153],"about_ca_topic_score_codex":0.012733182,"about_ca_topic_score_gemma":0.029957185,"teacher_disagreement_score":0.019336503,"about_ca_system_score_codex":0.00057638536,"about_ca_system_score_gemma":0.00015427185,"threshold_uncertainty_score":0.06468701},"labels":[],"label_agreement":null},{"id":"W4384929023","doi":"10.3847/1538-4357/acdb6a","title":"FAST Polarization Mapping of the Supernova Remnant VRO 42.05.01","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Supernova remnant; Faraday effect; Polarization (electrochemistry); Astrophysics; Galactic plane; Telescope; Magnetic field; Faraday cage; Stars; Supernova","score_opus":0.01235733412785734,"score_gpt":0.217522179124991,"score_spread":0.20516484499713367,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384929023","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9899093,0.00013518124,0.0014875914,0.00006165989,0.000012484009,0.000009126173,0.0030398553,0.00017628718,0.005168555],"genre_scores_gemma":[0.9890591,0.00006905797,0.0027271863,0.000023689197,0.000014839852,0.000008353988,0.007147238,0.00003521261,0.0009153064],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998536,0.0000107355345,0.000004146625,0.000028794842,0.000065206,0.000037416918],"domain_scores_gemma":[0.99971884,0.000029186956,0.000034922752,0.00003936504,0.00012640665,0.00005122011],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027076917,0.00023827598,0.00020211536,0.0012959396,0.00033496317,0.00045795547,0.00019093255,0.00015472058,0.0010517476],"category_scores_gemma":[0.0003339056,0.00017177664,0.00020523964,0.0010175447,0.00013226415,0.00011877698,0.0003606456,0.00019962403,0.00044354537],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011106908,0.00014556607,0.46398374,0.000116748204,0.00018742192,0.0025419784,0.0011143512,0.009229609,0.42368886,0.001665358,0.0054012868,0.0908143],"study_design_scores_gemma":[0.000019035178,0.000086245906,0.9711689,0.000010796558,0.00003056649,0.00051227363,0.00020823388,0.0040721893,0.0153237935,0.00017309783,0.008367863,0.000026880769],"about_ca_topic_score_codex":0.016597021,"about_ca_topic_score_gemma":0.022687346,"teacher_disagreement_score":0.016597021,"about_ca_system_score_codex":0.00032140894,"about_ca_system_score_gemma":0.00026593576,"threshold_uncertainty_score":0.033000827},"labels":[],"label_agreement":null},{"id":"W4384936771","doi":"10.3847/1538-4357/acdbc6","title":"JADES Imaging of GN-z11: Revealing the Morphology and Environment of a Luminous Galaxy 430 Myr after the Big Bang","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":159,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Herzberg Institute of Astrophysics","funders":"University of California, Santa Cruz; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Redshift; Astronomy; Surface brightness; Population; Star formation; Stellar population; Spectral energy distribution; Stellar mass","score_opus":0.007468658170949825,"score_gpt":0.19937257853031773,"score_spread":0.1919039203593679,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384936771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99658597,0.00011851917,0.00052044546,0.000070677954,0.000011203499,0.00000806593,0.0006197347,0.00007481286,0.001990606],"genre_scores_gemma":[0.99631065,0.00006954327,0.0010129556,0.000054628043,0.000014644151,0.0000054807156,0.00127648,0.00002233682,0.0012333494],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999385,0.000003321954,0.0000023692849,0.000016868167,0.00001783888,0.000021046735],"domain_scores_gemma":[0.9997769,0.000012001754,0.00005354329,0.000023035445,0.000043749045,0.00009082709],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016803172,0.00022148226,0.00018941521,0.00067107414,0.00036571795,0.00042265953,0.00023779462,0.00028375103,0.00105592],"category_scores_gemma":[0.00022872248,0.00018383769,0.00029303404,0.000259093,0.00021255836,0.00022002008,0.0004625939,0.00033200582,0.00039430487],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042939783,0.00015387067,0.6746531,0.0001283888,0.00015071765,0.001874417,0.0007481232,0.0015165332,0.29744747,0.0006116775,0.002961735,0.019324511],"study_design_scores_gemma":[0.0000039791394,0.000029946556,0.9957903,0.000005311779,0.000013286282,0.00025221772,0.00006775263,0.00049763656,0.0021371641,0.00002879413,0.0011689353,0.0000046589184],"about_ca_topic_score_codex":0.0073191994,"about_ca_topic_score_gemma":0.01758465,"teacher_disagreement_score":0.0073191994,"about_ca_system_score_codex":0.00061130535,"about_ca_system_score_gemma":0.00014594117,"threshold_uncertainty_score":0.014553189},"labels":[],"label_agreement":null},{"id":"W4384963985","doi":"10.3847/1538-4357/acd4c1","title":"Properties of Binary Systems in a One-dimensional Approximation","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Subgiant; Binary star; Stellar evolution; Binary number; Stars; Astrophysics; Roche lobe; Equipotential; Stellar mass; Asteroseismology; Star formation; Quantum mechanics","score_opus":0.02833854529416548,"score_gpt":0.22238418263359072,"score_spread":0.19404563733942523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4384963985","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9289693,0.00066616945,0.04107083,0.00015736697,0.00003651646,0.000027388454,0.0005671728,0.0002999327,0.028205253],"genre_scores_gemma":[0.9943779,0.0001167926,0.0042825933,0.000014115183,0.000010047562,0.000016573056,0.00024064045,0.000035054924,0.00090627413],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998487,0.000032705495,0.000012543678,0.000021063861,0.00005873934,0.000026219299],"domain_scores_gemma":[0.9992829,0.00035990254,0.00009594779,0.00006800064,0.00013456696,0.000058723177],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032950655,0.00019284654,0.0003483516,0.0010014323,0.00054883014,0.0010650677,0.00036715143,0.00034172577,0.0022790744],"category_scores_gemma":[0.0018682115,0.00016430291,0.00027633304,0.00062256714,0.0005117662,0.0005781904,0.0004271507,0.00029366498,0.00031883252],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006330285,0.00004739564,0.016827296,0.00011950906,0.000038551272,0.00022527768,0.00019435826,0.87171614,0.008201402,0.09224706,0.0009510186,0.009368738],"study_design_scores_gemma":[0.000006867487,0.000015766605,0.004754963,0.000010396313,0.000006592335,0.00007302275,0.000024088937,0.9821415,0.0014626419,0.010592267,0.0009027775,0.000009187777],"about_ca_topic_score_codex":0.002482593,"about_ca_topic_score_gemma":0.000902144,"teacher_disagreement_score":0.002482593,"about_ca_system_score_codex":0.00054509734,"about_ca_system_score_gemma":0.00029393556,"threshold_uncertainty_score":0.0076242685},"labels":[],"label_agreement":null},{"id":"W4385069994","doi":"10.3847/1538-4357/acc8d3","title":"The Spatial Clustering of ROSAT All-Sky Survey Active Galactic Nuclei. V. The Evolution of Broad-line AGN Clustering Properties in the Last 6 Gyr","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Leibniz-Institut für Astrophysik Potsdam; Ministério da Ciência, Tecnologia e Inovação; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Deutsche Forschungsgemeinschaft; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Bundesministerium für Bildung und Forschung; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Max-Planck-Gesellschaft; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; University of California, San Diego; Yale University; Max-Planck-Institut für Astrophysik","keywords":"ROSAT; Physics; Astrophysics; Sky; Astronomy; Active galactic nucleus; Cluster analysis; Line (geometry); Galaxy","score_opus":0.020857661290128955,"score_gpt":0.23596465173862902,"score_spread":0.21510699044850007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385069994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99800295,0.00014494579,0.00010692781,0.000035500514,0.000002319388,0.0000022235567,0.0010477284,0.000018888213,0.00063858443],"genre_scores_gemma":[0.9984659,0.000030248182,0.0000747541,0.000006321327,0.000002224446,0.0000015251157,0.0011018583,0.000005531482,0.00031163738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989367,0.000014091515,0.0000068488,0.000037730453,0.000024019582,0.00002358339],"domain_scores_gemma":[0.99888355,0.000094751485,0.00051327224,0.00007868542,0.0002443499,0.00018547937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029981177,0.00011541331,0.00011149882,0.0006672483,0.00016650268,0.0004532287,0.00018691849,0.00019158745,0.0009947399],"category_scores_gemma":[0.0011466099,0.00008074565,0.00019125287,0.0005591036,0.00017378623,0.00021785454,0.0003069282,0.00013026637,0.000421326],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000017508535,0.000005060335,0.99671495,0.000004020129,0.000027034112,0.000020377598,0.000058186775,0.0005681918,0.00079608127,0.000056495446,0.0002399183,0.0014921443],"study_design_scores_gemma":[3.1449906e-7,0.0000041046724,0.99935704,0.0000010292533,0.0000022726485,0.000012573947,0.000036330282,0.00036524568,0.00006802775,0.000008067096,0.00014392743,0.0000010207295],"about_ca_topic_score_codex":0.03381356,"about_ca_topic_score_gemma":0.037285887,"teacher_disagreement_score":0.03381356,"about_ca_system_score_codex":0.00050841406,"about_ca_system_score_gemma":0.00017087717,"threshold_uncertainty_score":0.0672335},"labels":[],"label_agreement":null},{"id":"W4385214769","doi":"10.3847/1538-4357/acd9cf","title":"A Spatially Resolved Analysis of Star Formation Burstiness by Comparing UV and Hα in Galaxies at z ∼ 1 with UVCANDELS","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Galaxy; Star formation; Stellar mass; Surface brightness; Initial mass function; Astronomy","score_opus":0.010692506734599766,"score_gpt":0.21505748852289105,"score_spread":0.2043649817882913,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385214769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99946827,0.00002150579,0.00011113756,0.000003305312,3.4616863e-7,0.0000014675655,0.00022624694,0.000010386308,0.00015724933],"genre_scores_gemma":[0.99908483,0.000013415266,0.00017334727,0.0000038131834,0.0000021681844,0.0000017191742,0.00064211723,0.0000032070745,0.000075384516],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998399,0.00001646241,0.000012010892,0.00005872185,0.000037269576,0.000035503774],"domain_scores_gemma":[0.9991768,0.000104882914,0.00035175344,0.00009628141,0.00009066253,0.00017960771],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027718823,0.00018219819,0.00024326322,0.0019345409,0.00018446347,0.00060286757,0.0002313992,0.0001839257,0.0007839088],"category_scores_gemma":[0.00064614415,0.00018471076,0.00028380516,0.0011264521,0.00019191855,0.00027362566,0.00049758353,0.00016152485,0.0002496837],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000074107804,0.000023874396,0.98762614,0.0000068276154,0.000079311816,0.000037382768,0.0001463349,0.00033638382,0.008279805,0.000044867753,0.00006615568,0.003278789],"study_design_scores_gemma":[8.19087e-7,0.000010354097,0.9994702,6.044351e-7,0.000007103953,0.000017930553,0.000041868,0.00019208471,0.00021726728,0.000008044668,0.000032980308,8.229793e-7],"about_ca_topic_score_codex":0.0064655114,"about_ca_topic_score_gemma":0.009121929,"teacher_disagreement_score":0.0064655114,"about_ca_system_score_codex":0.00022111493,"about_ca_system_score_gemma":0.00008537255,"threshold_uncertainty_score":0.012855768},"labels":[],"label_agreement":null},{"id":"W4385219597","doi":"10.3847/1538-4357/acdac8","title":"Not So Fast, Not So Furious: Just Magnetic","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; White dwarf; Stars; Supernova; Spectral line; Rotation period; Astronomy; Stellar rotation; Star (game theory); Radial velocity; Spectroscopy","score_opus":0.01690898072321239,"score_gpt":0.24013347831264797,"score_spread":0.22322449758943558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385219597","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5424786,0.0098616555,0.0078015057,0.12363195,0.010458943,0.000070848684,0.0007847382,0.00090974115,0.304002],"genre_scores_gemma":[0.9280222,0.0013367584,0.0018985664,0.016437674,0.00097107544,0.000011712735,0.0001657682,0.00012610907,0.051030144],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9991825,0.00020411504,0.00004733493,0.00016792977,0.00023288825,0.00016530324],"domain_scores_gemma":[0.9962915,0.0004859272,0.000784325,0.0005409708,0.0010331642,0.00086406746],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001027244,0.0002527936,0.00031018318,0.00048929104,0.001621234,0.0030604359,0.0004383589,0.0011554026,0.006947127],"category_scores_gemma":[0.0046641687,0.00019723504,0.00016834908,0.00033494565,0.0030659153,0.002808951,0.0012628819,0.0014073732,0.0029733004],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013675462,0.00027862456,0.279618,0.0010642536,0.00038299154,0.005881029,0.01376706,0.00051126425,0.038530294,0.099554956,0.3012629,0.25778112],"study_design_scores_gemma":[0.000071580966,0.0005652833,0.13589357,0.00058035715,0.00017476491,0.011043508,0.016443703,0.00065994624,0.007894423,0.050469063,0.77606297,0.00014086091],"about_ca_topic_score_codex":0.0024781052,"about_ca_topic_score_gemma":0.004889418,"teacher_disagreement_score":0.006947127,"about_ca_system_score_codex":0.0011428958,"about_ca_system_score_gemma":0.0009310969,"threshold_uncertainty_score":0.023240447},"labels":[],"label_agreement":null},{"id":"W4385305774","doi":"10.3847/1538-4357/acdc98","title":"The Radio Parallax of the Crab Pulsar: A First VLBI Measurement Calibrated with Giant Pulses","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"Joint Research Fund for Overseas Chinese Scholars and Scholars in Hong Kong and Macao; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Killam Trusts; Ministry of Science and Technology, Taiwan; University of Toronto; Government of Ontario; National Natural Science Foundation of China; National Radio Astronomy Observatory; Ontario Research Foundation; Canadian Institute for Advanced Research; Alexander von Humboldt-Stiftung; Vetenskapsrådet; National Science Foundation","keywords":"Physics; Very-long-baseline interferometry; Parallax; Crab Nebula; Astrometry; Pulsar; Astrophysics; Crab Pulsar; Astronomy; Calibration; Proper motion; Stars","score_opus":0.018416621564242407,"score_gpt":0.27267692643887287,"score_spread":0.25426030487463047,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385305774","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9860523,0.0004119654,0.0060140304,0.00015014564,0.000024471618,0.00003332539,0.0015509049,0.0004557789,0.005307163],"genre_scores_gemma":[0.9897625,0.00008850444,0.0066694277,0.00007559148,0.000023518736,0.000024768775,0.002341138,0.000088810775,0.0009258479],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997297,0.000029970812,0.000011832062,0.00007809571,0.00008539388,0.00006492571],"domain_scores_gemma":[0.9991761,0.00010440879,0.00015854531,0.00017254369,0.00023945633,0.00014901541],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005009362,0.00026573223,0.00035043544,0.0016594296,0.00047363283,0.00067668234,0.0005186173,0.00049899326,0.0012337486],"category_scores_gemma":[0.0011852087,0.00030642035,0.000239819,0.00079263083,0.0002394475,0.00040410113,0.00087543187,0.0006797506,0.00078866753],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00050029927,0.00029971803,0.6705688,0.00012179241,0.0002379829,0.00071362377,0.0007171878,0.0038049605,0.25892743,0.0006900793,0.0035758822,0.059842296],"study_design_scores_gemma":[0.000028799153,0.00019875434,0.9618827,0.0000218827,0.00005663974,0.0003763366,0.00011469204,0.0039738533,0.026732061,0.00016100668,0.006420052,0.00003330841],"about_ca_topic_score_codex":0.005268406,"about_ca_topic_score_gemma":0.007819125,"teacher_disagreement_score":0.005268406,"about_ca_system_score_codex":0.000649276,"about_ca_system_score_gemma":0.0002866299,"threshold_uncertainty_score":0.010475457},"labels":[],"label_agreement":null},{"id":"W4385327525","doi":"10.3847/1538-4357/ad05cd","title":"The Atacama Cosmology Telescope: Galactic Dust Structure and the Cosmic PAH Background in Cross-correlation with WISE","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Institute of Standards and Technology; Fondo Nacional de Desarrollo Científico y Tecnológico; National Aeronautics and Space Administration; Agencia Nacional de Investigación y Desarrollo; University of Pennsylvania; Princeton University; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Cosmology; Cosmic infrared background; Power law; Cosmic microwave background; Cosmic background radiation; Spectral index; Milky Way; Galaxy; Spectral line","score_opus":0.0052337970920718286,"score_gpt":0.23933441558803228,"score_spread":0.23410061849596045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385327525","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965699,0.00008197856,0.0011694913,0.000046356017,0.000008195349,0.000004855422,0.00066892104,0.000056622546,0.001393664],"genre_scores_gemma":[0.99765366,0.000023358756,0.0005409309,0.000026042799,0.00001572459,0.000004820784,0.0013215784,0.0000314801,0.00038236272],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992786,0.00017313124,0.000028062243,0.00019764081,0.00021969926,0.00010286516],"domain_scores_gemma":[0.9959747,0.0011043202,0.0011329766,0.0005901987,0.00053062214,0.0006671595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011539959,0.00030261918,0.00031004363,0.0018126597,0.00037490175,0.00096327707,0.00044005347,0.0003118609,0.00155799],"category_scores_gemma":[0.002908315,0.0002028993,0.00043566982,0.0022542956,0.00041888515,0.00034725625,0.0007521197,0.00041852792,0.00039576585],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000767268,0.000035679404,0.991454,0.000006627558,0.00016092008,0.000118643824,0.00009675857,0.0007971461,0.0034915954,0.00021699934,0.0006757505,0.0028691527],"study_design_scores_gemma":[0.0000013845927,0.000007952098,0.9979557,0.000001019199,0.000012497168,0.000037454716,0.000023282992,0.0013669643,0.00036067885,0.000032345983,0.00019789049,0.0000029018586],"about_ca_topic_score_codex":0.014620059,"about_ca_topic_score_gemma":0.016298968,"teacher_disagreement_score":0.014620059,"about_ca_system_score_codex":0.00033088535,"about_ca_system_score_gemma":0.00024233841,"threshold_uncertainty_score":0.02906996},"labels":[],"label_agreement":null},{"id":"W4385340275","doi":"10.3847/1538-4357/acdee3","title":"A Recipe for Unbiased Background Modeling in Deep Wide-field Astronomical Images","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Physics; Sky; Sky brightness; Telescope; Astronomy; Galaxy; Cirrus; Large Synoptic Survey Telescope; Photometry (optics); Brightness; Surface brightness; Field of view; Remote sensing; Astrophysics; Optics; Stars","score_opus":0.023152207327137755,"score_gpt":0.2507496086268265,"score_spread":0.22759740129968875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385340275","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0014213658,0.000023639272,0.9977805,0.000044581728,0.000010998902,0.000016552109,0.00005796465,0.00046800313,0.00017651812],"genre_scores_gemma":[0.032162283,0.00008307823,0.9654862,0.000097536074,0.00005794173,0.0001206654,0.00045171156,0.0005041153,0.0010363464],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9989693,0.00027752478,0.00007162258,0.00022599493,0.00034218887,0.00011341068],"domain_scores_gemma":[0.9974087,0.0009304484,0.0002666532,0.00065295,0.00058590097,0.00015530206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0031466987,0.0010771377,0.0011208605,0.0018975503,0.0009135076,0.002165253,0.0029868847,0.0012873312,0.0040018097],"category_scores_gemma":[0.008040711,0.0011719682,0.0016955168,0.0015206214,0.0010812094,0.0018586374,0.0025123046,0.0026514148,0.002579531],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021205886,0.00019285582,0.0053985636,0.00026959748,0.00028874527,0.0004909472,0.00037568389,0.4301774,0.05951913,0.159217,0.011073481,0.3327846],"study_design_scores_gemma":[0.000012131967,0.000019734991,0.00071842317,0.000017510414,0.000019191562,0.00008259822,0.000026286647,0.9458923,0.007285657,0.040953003,0.0049309353,0.000042177388],"about_ca_topic_score_codex":0.0063344114,"about_ca_topic_score_gemma":0.010616469,"teacher_disagreement_score":0.0063344114,"about_ca_system_score_codex":0.0010321504,"about_ca_system_score_gemma":0.0013970248,"threshold_uncertainty_score":0.016641498},"labels":[],"label_agreement":null},{"id":"W4385340757","doi":"10.3847/1538-4357/acdf4f","title":"Characterizing the Spectral Structure of Weak Impulsive Narrowband Quiet Sun Emissions","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"National Science Foundation","keywords":"Physics; Narrowband; Astrophysics; QUIET; Nanoflares; Flux (metallurgy); Corona (planetary geology); Astronomy; Coronal hole; Radio spectrum; Coronal mass ejection; Solar wind; Plasma; Optics; Astrobiology","score_opus":0.006240540001638413,"score_gpt":0.2334822694239421,"score_spread":0.2272417294223037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385340757","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956145,0.00018762489,0.0022866558,0.000019399906,0.000005393086,0.000006765252,0.00023116694,0.000039090533,0.0016094097],"genre_scores_gemma":[0.9988801,0.000045371882,0.00049702,0.00000887507,0.0000067163546,0.0000034354298,0.00035019303,0.000009055917,0.00019934063],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992156,0.00000708416,0.0000058937635,0.000025419075,0.000019775582,0.000020324944],"domain_scores_gemma":[0.9993869,0.00018660908,0.0001815609,0.00004178183,0.0001011389,0.00010197424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023030439,0.000117714284,0.00015851813,0.0015155842,0.00013958682,0.00042849078,0.00018965919,0.00016388265,0.0012090742],"category_scores_gemma":[0.0007449974,0.0000909381,0.00011250616,0.0004928605,0.00018865654,0.00032985132,0.0003804615,0.00013524917,0.00024499078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004090221,0.000048480968,0.7910578,0.00012496843,0.000102384714,0.00043860558,0.00047421383,0.0014277663,0.17283885,0.001027928,0.0005504196,0.03149944],"study_design_scores_gemma":[0.000006215496,0.000056425648,0.99067616,0.000008108266,0.000020950209,0.00030126947,0.00018244793,0.002437696,0.0051224185,0.00039321545,0.0007865903,0.000008612819],"about_ca_topic_score_codex":0.00037280683,"about_ca_topic_score_gemma":0.0006117664,"teacher_disagreement_score":0.0015155842,"about_ca_system_score_codex":0.00009593559,"about_ca_system_score_gemma":0.00003514065,"threshold_uncertainty_score":0.004044771},"labels":[],"label_agreement":null},{"id":"W4385340966","doi":"10.3847/1538-4357/acdb6f","title":"The Inner 2 pc of Sagittarius A*: Simulations of the Circumnuclear Disk and Multiphase Gas Accretion in the Galactic Center","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Physics; Galactic Center; Astrophysics; Accretion (finance); Supermassive black hole; Sagittarius A*; Milky Way; Star cluster; Astronomy; Stars; Gravitational potential; Galaxy","score_opus":0.014500903379822986,"score_gpt":0.2485943948545669,"score_spread":0.23409349147474393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385340966","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99340993,0.00008974486,0.00050944154,0.00017233404,0.0000212224,0.00001599606,0.00037118656,0.00010769465,0.005302366],"genre_scores_gemma":[0.9980259,0.000054140808,0.00072998635,0.000072819,0.000008282627,0.000015998576,0.0004147353,0.0000409476,0.00063712144],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998921,0.000024179577,0.000004433294,0.000020077121,0.000018855819,0.000040412117],"domain_scores_gemma":[0.99961865,0.00012243447,0.000037744223,0.00002486532,0.00006421733,0.00013196272],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021056521,0.0004578376,0.00053158595,0.0004045941,0.0008404981,0.0010713056,0.001381312,0.0011363882,0.0029051017],"category_scores_gemma":[0.00085674843,0.00031164155,0.0004989452,0.00049214833,0.0007982475,0.0004136192,0.0008634408,0.0006810783,0.00031732843],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037852264,0.00040144913,0.02555299,0.000058218637,0.0001577407,0.0005017183,0.0002553016,0.9614005,0.0027917002,0.003192547,0.0021606046,0.0031486193],"study_design_scores_gemma":[0.00015880892,0.00012642829,0.009228396,0.000013236569,0.000028172568,0.000036775895,0.00021384715,0.98792344,0.00059239654,0.0005839733,0.0010768652,0.000017790055],"about_ca_topic_score_codex":0.075919695,"about_ca_topic_score_gemma":0.038666885,"teacher_disagreement_score":0.075919695,"about_ca_system_score_codex":0.0015394877,"about_ca_system_score_gemma":0.0010044293,"threshold_uncertainty_score":0.15095556},"labels":[],"label_agreement":null},{"id":"W4385408926","doi":"10.3847/1538-4357/acdc90","title":"X-Ray Properties of Optically Variable Low-mass AGN Candidates","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Smithsonian Astrophysical Observatory; University of Portsmouth; University of California, Los Angeles; York University; Space Telescope Science Institute; Carnegie Mellon University; Office of Science; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Jet Propulsion Laboratory; Gordon and Betty Moore Foundation; New Mexico State University; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Observatory; Astronomy; X-ray","score_opus":0.007750152823427363,"score_gpt":0.19567483181542153,"score_spread":0.18792467899199417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385408926","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99974173,0.000031374613,0.000047941554,0.0000031407646,3.5841282e-7,0.0000015013264,0.000031947777,0.0000028108238,0.00013915372],"genre_scores_gemma":[0.99961627,0.000010921007,0.000060926603,0.0000037669786,0.0000022430313,0.0000016051594,0.00016094881,0.000001271077,0.00014206732],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998561,0.000023957438,0.000012356155,0.000034636643,0.00003203372,0.000040794348],"domain_scores_gemma":[0.9988158,0.0002740279,0.00046504487,0.000068035784,0.00013155001,0.0002454841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033471163,0.00023203791,0.00031251568,0.0016465364,0.00032475241,0.00071645086,0.00030967494,0.00022609695,0.0015113421],"category_scores_gemma":[0.0009641139,0.000099829354,0.00016019701,0.00060818234,0.00032679076,0.0002194002,0.0003705492,0.00014228349,0.00041832228],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014621044,0.00004394524,0.9874922,0.0000071088366,0.000015259935,0.0001380185,0.000107588814,0.00009462048,0.009919755,0.000033207187,0.000031778967,0.0019702397],"study_design_scores_gemma":[0.000003276905,0.000054836946,0.9984491,0.0000015554101,0.000009691008,0.0001994746,0.00008201065,0.000227567,0.00087461213,0.000014717924,0.00008145839,0.0000017854373],"about_ca_topic_score_codex":0.001297324,"about_ca_topic_score_gemma":0.0014499733,"teacher_disagreement_score":0.0016465364,"about_ca_system_score_codex":0.00017855557,"about_ca_system_score_gemma":0.00005630764,"threshold_uncertainty_score":0.0050559044},"labels":[],"label_agreement":null},{"id":"W4385429454","doi":"10.3847/1538-4357/acdd57","title":"Active Galactic Nuclei Feedback in SDSS-IV MaNGA: AGNs Have Suppressed Central Star Formation Rates","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Berkeley National Laboratory; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Star formation; Active galactic nucleus; Galaxy; Redshift; Astronomy; Galaxy formation and evolution","score_opus":0.010873377589718737,"score_gpt":0.2283688676037908,"score_spread":0.21749549001407206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385429454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99945134,0.00003261303,0.00012946322,0.000012317545,0.0000013640398,0.000001147741,0.00014927868,0.000019976444,0.00020255135],"genre_scores_gemma":[0.99957544,0.0000062945064,0.00007320696,0.0000073511815,0.0000017641489,0.0000010248674,0.00021639824,0.000004044189,0.000114541224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989057,0.000010853246,0.0000057597194,0.000046567693,0.000017441584,0.000028935034],"domain_scores_gemma":[0.9992699,0.00009392876,0.0002589329,0.00010851771,0.00008191518,0.00018671078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002953936,0.00017864072,0.0002828419,0.0004783595,0.00026660037,0.00040015325,0.00021802762,0.00014587579,0.0010248144],"category_scores_gemma":[0.00061957136,0.00013196054,0.00020632586,0.0002708526,0.00042360663,0.00020722211,0.00031675564,0.00020761568,0.0002702995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020139758,0.000045175148,0.9387177,0.000017992601,0.000055798282,0.00014009504,0.00019236561,0.00060029555,0.056682404,0.00015033632,0.00012319902,0.0030731875],"study_design_scores_gemma":[0.0000027126212,0.000019228495,0.99791497,0.0000012822744,0.0000063646767,0.00003641936,0.000038922393,0.0007194593,0.0011041124,0.000049805574,0.00010464392,0.0000020251405],"about_ca_topic_score_codex":0.0062035345,"about_ca_topic_score_gemma":0.0081358645,"teacher_disagreement_score":0.0062035345,"about_ca_system_score_codex":0.00039634109,"about_ca_system_score_gemma":0.00013094136,"threshold_uncertainty_score":0.012334824},"labels":[],"label_agreement":null},{"id":"W4385461387","doi":"10.3847/1538-4357/acd53c","title":"First Sample of Hα+[O iii]λ5007 Line Emitters at z &gt; 6 Through JWST/NIRCam Slitless Spectroscopy: Physical Properties and Line-luminosity Functions","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":82,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"European Research Council; European Commission; Science and Technology Facilities Council; Space Telescope Science Institute; University of Arizona; National Aeronautics and Space Administration","keywords":"Physics; Line (geometry); Luminosity; Spectroscopy; Emission spectrum; Astrophysics; Astronomy; Spectral line; Galaxy","score_opus":0.020543644715972382,"score_gpt":0.2300914381210879,"score_spread":0.2095477934051155,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385461387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989139,0.000044196644,0.00013565636,0.000010250437,0.000001352466,0.00000921011,0.00050892535,0.000011833835,0.0003647079],"genre_scores_gemma":[0.99606687,0.000051258106,0.00041980308,0.000033602457,0.000013472379,0.000009636524,0.002649005,0.0000085825,0.0007478769],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977106,0.000013145895,0.000014985147,0.000052843534,0.00006742657,0.00008045176],"domain_scores_gemma":[0.999451,0.000048799913,0.00009971706,0.00006386628,0.00012244709,0.00021418605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021464098,0.00027911193,0.00034991297,0.0014888736,0.0005658967,0.0005586841,0.00038270123,0.0002583013,0.0015905595],"category_scores_gemma":[0.00037304984,0.00017701635,0.00023738187,0.00064367056,0.00021089573,0.000357019,0.000624642,0.0002820303,0.00077173946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016224237,0.00027481455,0.96326506,0.000016323573,0.000042926735,0.00050200487,0.00049860956,0.000060078706,0.024602616,0.000084967214,0.000498017,0.009992432],"study_design_scores_gemma":[0.0000046251157,0.000061039915,0.9975776,0.0000023670634,0.000015284126,0.00027342577,0.00012372548,0.0001014962,0.0010489275,0.000015039192,0.0007735963,0.0000029390446],"about_ca_topic_score_codex":0.0056833196,"about_ca_topic_score_gemma":0.009863092,"teacher_disagreement_score":0.0056833196,"about_ca_system_score_codex":0.00020850204,"about_ca_system_score_gemma":0.0001607474,"threshold_uncertainty_score":0.011300504},"labels":[],"label_agreement":null},{"id":"W4385461592","doi":"10.3847/1538-4357/ace1ee","title":"AT 2021loi: A Bowen Fluorescence Flare with a Rebrightening Episode Occurring in a Previously Known AGN","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Planning and Budgeting Committee of the Council for Higher Education of Israel; Agencia Nacional de Investigación y Desarrollo; Science and Technology Facilities Council; National Development and Reform Commission; Canadian Institute for Advanced Research; United States-Israel Binational Science Foundation; Israel Science Foundation; Council for Higher Education; European Commission; Chinese Academy of Sciences; John Templeton Foundation; National Aeronautics and Space Administration; European Research Council; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Supermassive black hole; Astronomy; Galaxy; Flare; Light curve; Active galactic nucleus; Accretion (finance); Observatory","score_opus":0.012371712615075808,"score_gpt":0.23296056433860193,"score_spread":0.22058885172352613,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385461592","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9941859,0.000102274775,0.0002676666,0.00014061306,0.00002408813,0.000024298297,0.0007866956,0.0000515233,0.004416941],"genre_scores_gemma":[0.9969958,0.000042277657,0.00032400308,0.00011575513,0.00004597212,0.000010143628,0.0011595453,0.000009085088,0.0012975408],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998909,0.0000025317229,0.0000028755287,0.000021639544,0.000022258148,0.00005970609],"domain_scores_gemma":[0.99974936,0.000014640784,0.000063572894,0.000015307922,0.000030121093,0.00012702236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011221078,0.0002469603,0.00027238927,0.0010507201,0.0010945227,0.0004755213,0.0002768003,0.0007167312,0.0020768186],"category_scores_gemma":[0.00022037805,0.00012263622,0.0002092018,0.00056304736,0.00016226056,0.00029870452,0.00053613255,0.00054969237,0.00057477795],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000554392,0.00044620613,0.8375959,0.00011354934,0.00006987983,0.02499736,0.001802325,0.00055167824,0.09530655,0.0004143247,0.0058330833,0.03231484],"study_design_scores_gemma":[0.0000049490436,0.0001593152,0.99028206,0.000013641754,0.000012672694,0.0042196335,0.00033648507,0.0002965149,0.0014991597,0.00005635642,0.003107629,0.000011495398],"about_ca_topic_score_codex":0.010486805,"about_ca_topic_score_gemma":0.023293894,"teacher_disagreement_score":0.010486805,"about_ca_system_score_codex":0.0006187936,"about_ca_system_score_gemma":0.00015238265,"threshold_uncertainty_score":0.020851552},"labels":[],"label_agreement":null},{"id":"W4385493970","doi":"10.3847/1538-4357/acdedd","title":"Probing the Origin of Changing-look Quasar Transitions with Chandra","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Institut National de Physique Nucléaire et de Physique des Particules; Deutsches Elektronen-Synchrotron; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; National Central University; Max-Planck-Gesellschaft; Queen's University Belfast; Durham University; York University; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; Space Telescope Science Institute; Carnegie Mellon University; College of Engineering, Michigan State University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Harvard University; Queen's University; Ohio State University; Agencia Nacional de Investigación y Desarrollo; Trinity College Dublin; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; Stockholms Universitet; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Quasar; Supermassive black hole; Light curve; Accretion (finance); Spectral line; Astronomy; Flux (metallurgy); Emission spectrum; Amplitude; Spectral slope; Torus; Galaxy; Optics","score_opus":0.019244470768759823,"score_gpt":0.23789343754046013,"score_spread":0.21864896677170031,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385493970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978849,0.00011597234,0.0008072667,0.000030128436,0.000005946309,0.000010960847,0.00030474615,0.000040472514,0.00079950126],"genre_scores_gemma":[0.99912614,0.000022927687,0.000524072,0.000014477117,0.0000053969243,0.0000030755555,0.00020479473,0.0000060573266,0.000092973656],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997273,0.000028487355,0.000015439566,0.000078428035,0.00005746241,0.00009283834],"domain_scores_gemma":[0.99799687,0.0002811739,0.0007877749,0.00026908342,0.00021238538,0.00045269533],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051154016,0.00019588882,0.00017877703,0.0016430528,0.00046193314,0.0009652918,0.00034866575,0.00019436062,0.0011389111],"category_scores_gemma":[0.0010134358,0.00015220637,0.00028181312,0.0008125783,0.00036028028,0.00049070467,0.0007963143,0.00054683886,0.00016898468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013540158,0.00006663355,0.9700009,0.00002521687,0.000059123468,0.0004648379,0.00037606098,0.0001763832,0.020043297,0.0010325038,0.0003141451,0.0073053986],"study_design_scores_gemma":[0.000005284059,0.000041900785,0.99607384,0.0000060419034,0.000015437108,0.00039893592,0.00017968782,0.00066871726,0.0014702459,0.00028506096,0.00084602897,0.000008930343],"about_ca_topic_score_codex":0.002078184,"about_ca_topic_score_gemma":0.002676531,"teacher_disagreement_score":0.002078184,"about_ca_system_score_codex":0.00023315163,"about_ca_system_score_gemma":0.00015957287,"threshold_uncertainty_score":0.0041321516},"labels":[],"label_agreement":null},{"id":"W4385576496","doi":"10.3847/1538-4357/ace343","title":"PEARLS: Low Stellar Density Galaxies in the El Gordo Cluster Observed with JWST","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Chinese Academy of Sciences; National Natural Science Foundation of China; Agencia Estatal de Investigación; National Aeronautics and Space Administration; Ministerio de Ciencia, Innovación y Universidades; European Space Agency; Goddard Space Flight Center; Chinese Academy of Sciences South America Center for Astronomy; Nuclear Safety and Security Commission; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Galaxy; Surface brightness; Redshift; Brightness; Population; Astronomy; Cluster (spacecraft); Stellar population; Star formation; Medicine","score_opus":0.013367821261854498,"score_gpt":0.21363218623248334,"score_spread":0.20026436497062883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385576496","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993437,0.000016945884,0.000043672866,0.000013587422,7.744593e-7,0.0000025641934,0.00014061936,0.000009836103,0.0004282283],"genre_scores_gemma":[0.9991079,0.000015439804,0.00012257339,0.000015068597,0.0000018293049,0.000003616208,0.000377078,0.000006171614,0.00035034888],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991465,0.0000046235173,0.000003131676,0.000028525781,0.000021396776,0.000027667444],"domain_scores_gemma":[0.9997398,0.000021287571,0.00007383747,0.00002830678,0.00003360773,0.00010307687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001314845,0.00015589254,0.00027973825,0.0010629335,0.00041698292,0.0004692285,0.00034373492,0.00015576046,0.0011341124],"category_scores_gemma":[0.000358155,0.0001100203,0.00007995263,0.00047926203,0.0005030677,0.00022580977,0.0006865266,0.00018093215,0.00027835878],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011320517,0.0000343359,0.98341054,0.000021251113,0.000031701715,0.00027524823,0.00086096086,0.0001044866,0.010325231,0.00013905522,0.0005053372,0.0041785454],"study_design_scores_gemma":[0.0000022734032,0.000009368641,0.9990369,0.0000017893361,0.000004047889,0.000064650456,0.00033996248,0.000081417784,0.00014146866,0.000015810298,0.00030030368,0.0000019029916],"about_ca_topic_score_codex":0.033959966,"about_ca_topic_score_gemma":0.081507705,"teacher_disagreement_score":0.033959966,"about_ca_system_score_codex":0.00039994446,"about_ca_system_score_gemma":0.00014454048,"threshold_uncertainty_score":0.06752455},"labels":[],"label_agreement":null},{"id":"W4385616914","doi":"10.3847/1538-4357/acdc97","title":"Observed Polarized Scattered Light Phase Functions of Planet-forming Disks","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"BC Cancer Agency; Japan Society for the Promotion of Science; Office National d'études et de Recherches Aérospatiales; Max-Planck-Institut für Astronomie; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Eidgenössische Technische Hochschule Zürich; Centre National de la Recherche Scientifique; European Commission","keywords":"Physics; Planet; Exoplanet; Phase (matter); Astronomy; Astrobiology; Astrophysics","score_opus":0.032066208834412614,"score_gpt":0.2698442590436814,"score_spread":0.23777805020926882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385616914","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99610966,0.00008514758,0.0020125823,0.000016774582,0.0000030209264,0.0000050433914,0.0005655084,0.000056572168,0.0011458067],"genre_scores_gemma":[0.9985361,0.00003528184,0.00068067416,0.000005120586,0.0000037804937,0.000003645953,0.00060395274,0.000016829928,0.00011467392],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989724,0.000014680702,0.0000059336785,0.000026393178,0.000026657804,0.000028999597],"domain_scores_gemma":[0.99936324,0.00017899294,0.00008733474,0.00008786355,0.00020801777,0.0000745768],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019389823,0.00035637696,0.00022668559,0.0020837253,0.00028718493,0.000621862,0.00019488596,0.00023763254,0.0009700379],"category_scores_gemma":[0.00051946106,0.00018383803,0.00022229615,0.0008462882,0.0003528286,0.0003057932,0.00024479395,0.0002088592,0.00025430595],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015435362,0.0002580614,0.3545235,0.00016598494,0.00026502446,0.0008658358,0.00061270903,0.014778949,0.5809099,0.0021375716,0.001605326,0.04233356],"study_design_scores_gemma":[0.00003888995,0.00014640203,0.8658448,0.000017831131,0.000065340675,0.0009290234,0.00036589883,0.038243547,0.09166779,0.0011899989,0.0014489905,0.000041493113],"about_ca_topic_score_codex":0.0012783885,"about_ca_topic_score_gemma":0.0010534659,"teacher_disagreement_score":0.0020837253,"about_ca_system_score_codex":0.00027980172,"about_ca_system_score_gemma":0.000086253036,"threshold_uncertainty_score":0.0032451153},"labels":[],"label_agreement":null},{"id":"W4385630230","doi":"10.3847/1538-4357/ace04f","title":"Constraining the Evolution of the Unstable Accretion Disk in SMC X-1 with NICER","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Neutron star; Accretion (finance); Instability; Luminosity; Astronomy; Precession; Galaxy; Mechanics","score_opus":0.011962130269543734,"score_gpt":0.22345021047857408,"score_spread":0.21148808020903034,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385630230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994361,0.000031777017,0.000162986,0.0000057567445,0.0000011308094,0.0000022251386,0.000065457774,0.000007678724,0.0002869688],"genre_scores_gemma":[0.99905044,0.000021452972,0.0005291418,0.000009299441,0.0000035630503,0.000003679528,0.00024983461,0.00000627154,0.00012625998],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.000009016349,0.0000030879526,0.000023154013,0.000013383618,0.000014012247],"domain_scores_gemma":[0.99983454,0.000027192767,0.000060160757,0.000023674247,0.000024700927,0.000029671231],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025680877,0.00015833398,0.00017498927,0.0004886087,0.00029462043,0.00031646283,0.00023140362,0.00019576763,0.00044306534],"category_scores_gemma":[0.0002243107,0.00013232065,0.00013977783,0.0002619347,0.00015347677,0.00016246323,0.00031251184,0.00015401668,0.00010459404],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005452614,0.00014498258,0.41930887,0.000041897743,0.000088756,0.00035800747,0.0003227043,0.001296609,0.56656635,0.0002970784,0.00017993248,0.010849573],"study_design_scores_gemma":[0.000015692887,0.00013777323,0.96749216,0.0000050431163,0.000032633503,0.00016012287,0.000094576346,0.008521711,0.022871245,0.00008180203,0.000579199,0.000008065328],"about_ca_topic_score_codex":0.0016845416,"about_ca_topic_score_gemma":0.0040143426,"teacher_disagreement_score":0.0016845416,"about_ca_system_score_codex":0.00017404227,"about_ca_system_score_gemma":0.00009046154,"threshold_uncertainty_score":0.003349483},"labels":[],"label_agreement":null},{"id":"W4385664096","doi":"10.3847/1538-4357/ace4be","title":"Subhalo Spreading of Thin Tidal Star Streams","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Velocity dispersion; Globular cluster; STREAMS; Milky Way; Stars; Astronomy; Dark matter; Galaxy","score_opus":0.009300419063478428,"score_gpt":0.22043639147562163,"score_spread":0.2111359724121432,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385664096","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999419,0.000011188268,0.00028813924,0.000013494122,0.0000015249753,0.0000019692516,0.0000441934,0.00001648674,0.00020407011],"genre_scores_gemma":[0.9995326,0.000011376302,0.00018843406,0.0000071895056,0.0000014512918,0.0000019319498,0.000119598924,0.000006154532,0.00013127582],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999392,0.0000102651675,0.0000035969886,0.000018216842,0.000008313247,0.000020445916],"domain_scores_gemma":[0.9993345,0.00016974998,0.00011651623,0.00009625565,0.000089586414,0.00019341403],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021118527,0.00025693147,0.00028874158,0.00032038623,0.0003393358,0.0007081841,0.00044555234,0.00029042462,0.0009294938],"category_scores_gemma":[0.0013243424,0.00015951309,0.00035487692,0.00022548018,0.00038582427,0.00042607097,0.0005819358,0.00024797887,0.00012512424],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008017498,0.00022179383,0.351816,0.0000544532,0.00023873763,0.00050548953,0.00051585137,0.60396487,0.02674588,0.0037331088,0.0010026989,0.010399426],"study_design_scores_gemma":[0.00010488424,0.00022258864,0.18215303,0.000017058805,0.00007210506,0.00013364051,0.00034308585,0.80540967,0.008406385,0.0020217092,0.0010819676,0.000033936132],"about_ca_topic_score_codex":0.006162356,"about_ca_topic_score_gemma":0.003948389,"teacher_disagreement_score":0.006162356,"about_ca_system_score_codex":0.00048914814,"about_ca_system_score_gemma":0.00021597001,"threshold_uncertainty_score":0.012252927},"labels":[],"label_agreement":null},{"id":"W4385724146","doi":"10.3847/1538-4357/ace1e1","title":"Reprocessing Models for the Optical Light Curves of Hypervariable Quasars from the Sloan Digital Sky Survey Reverberation Mapping Project","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Quasar; Physics; Astrophysics; Sky; Light curve; Astronomy; Galaxy","score_opus":0.03408201487325872,"score_gpt":0.24942896316569174,"score_spread":0.215346948292433,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385724146","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97310084,0.00014908181,0.023068195,0.00025841477,0.00000948338,0.0000310564,0.0006955541,0.00027849467,0.0024089606],"genre_scores_gemma":[0.9954581,0.00006236455,0.0031318322,0.00001803342,0.0000066505304,0.00001555739,0.00071912265,0.000043357682,0.0005448696],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99969876,0.00009068714,0.00001669124,0.000081873,0.000050765175,0.000061279236],"domain_scores_gemma":[0.99810576,0.00058303244,0.00054671784,0.00032232213,0.00030375962,0.00013836485],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013838276,0.000558686,0.00030358176,0.0012379092,0.00037359132,0.0011896379,0.0010353664,0.00060950214,0.0016892714],"category_scores_gemma":[0.0035053934,0.00025729992,0.0009899178,0.0006859772,0.00054892356,0.00079555815,0.000584976,0.00045518982,0.00040619128],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001395974,0.00008090805,0.24880478,0.000041514853,0.00012833251,0.0004372313,0.0005119314,0.72072524,0.002750013,0.0089977,0.0015188926,0.015863864],"study_design_scores_gemma":[0.000015553587,0.000043500764,0.065577224,0.000013764559,0.000028601835,0.00014942947,0.00013134391,0.9267598,0.00068394496,0.005276495,0.0012983691,0.000021963358],"about_ca_topic_score_codex":0.0179898,"about_ca_topic_score_gemma":0.010374249,"teacher_disagreement_score":0.0179898,"about_ca_system_score_codex":0.0009810247,"about_ca_system_score_gemma":0.0003205604,"threshold_uncertainty_score":0.035770178},"labels":[],"label_agreement":null},{"id":"W4385795147","doi":"10.3847/1538-4357/ace185","title":"The Metal-weak Milky Way Stellar Disk Hidden in the Gaia–Sausage–Enceladus Debris: The APOGEE DR17 View","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; U.S. Department of Energy; Smithsonian Institution; Vetenskapsrådet; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Max-Planck-Institut für Astrophysik; Knut och Alice Wallenbergs Stiftelse; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Physics; Astrophysics; Thick disk; Milky Way; Stars; Astronomy; Galaxy; Halo; Galactic halo; Population","score_opus":0.017470032182793856,"score_gpt":0.24459131016324945,"score_spread":0.2271212779804556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385795147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99874914,0.0001357937,0.000079675214,0.000038558446,0.0000044242292,0.0000012320477,0.00008397341,0.000008641025,0.0008985377],"genre_scores_gemma":[0.9994555,0.000035680612,0.000094511,0.000021482065,0.0000066712787,0.0000010624982,0.00014356924,0.000007314678,0.0002342793],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999306,0.000006739448,0.0000037058535,0.000027276992,0.000011381635,0.000020340642],"domain_scores_gemma":[0.99966276,0.00003661022,0.000121680445,0.00004565759,0.000045463887,0.00008780527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017363683,0.00026775582,0.0003273389,0.0007686426,0.0004735847,0.0009013295,0.0002367788,0.0002358289,0.001294236],"category_scores_gemma":[0.00030724207,0.00013801765,0.0001815683,0.0004811445,0.0005096102,0.0002731497,0.0008320759,0.00020158419,0.0003936921],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002288379,0.000028119168,0.9527111,0.000045953897,0.00012261853,0.0010493691,0.000561528,0.00020507615,0.035601098,0.00037360485,0.00043528463,0.008637368],"study_design_scores_gemma":[0.00001012593,0.00005499834,0.99528766,0.000009701352,0.00003895305,0.0005033082,0.00052893435,0.0003332923,0.0012882784,0.00016037111,0.0017799361,0.0000043985265],"about_ca_topic_score_codex":0.0026868926,"about_ca_topic_score_gemma":0.0049289637,"teacher_disagreement_score":0.0026868926,"about_ca_system_score_codex":0.00035400596,"about_ca_system_score_gemma":0.0001584888,"threshold_uncertainty_score":0.005342543},"labels":[],"label_agreement":null},{"id":"W4385813388","doi":"10.3847/1538-4357/ace342","title":"Continuum Reverberation Mapping of Mrk 876 over Three Years with Remote Robotic Observatories","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Science and Technology Facilities Council; Planetary Science Division; Science Mission Directorate; University of California, Irvine; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Gordon and Betty Moore Foundation; National Central University; Space Telescope Science Institute; Queen's University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Reverberation mapping; Amplitude; Astrophysics; RADIUS; Lag; Light curve; Wavelength; Active galactic nucleus; Normalization (sociology); Flux (metallurgy); Astronomy; Optics; Galaxy","score_opus":0.019141845624346086,"score_gpt":0.23426687817429853,"score_spread":0.21512503254995244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385813388","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981742,0.00005635871,0.000403821,0.0000235564,0.000005327228,0.000006343095,0.00049916696,0.000051183324,0.00077997707],"genre_scores_gemma":[0.9973363,0.000027714259,0.0008723183,0.000019205876,0.000012135021,0.000006322262,0.0011645422,0.000021339996,0.0005401535],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996996,0.000024830839,0.000013769963,0.0000880973,0.000105286636,0.00006841143],"domain_scores_gemma":[0.99905926,0.00006961479,0.0003267274,0.00014376327,0.00024971392,0.00015097504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042174556,0.00027653464,0.0003117735,0.00095304765,0.00046240498,0.00042978782,0.00034022675,0.0002534986,0.0007486149],"category_scores_gemma":[0.0006165498,0.00014440162,0.00026551797,0.00061878236,0.00022230421,0.00028998303,0.0007067517,0.00035411885,0.000474337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000609724,0.0003301439,0.8824774,0.00006277599,0.00019135092,0.00088998536,0.00092240016,0.0023590755,0.06931762,0.00018213579,0.0013568358,0.0413005],"study_design_scores_gemma":[0.0000033080657,0.000063731415,0.9969229,0.000002247682,0.000012198342,0.00010945411,0.00007080738,0.00061008,0.0014371166,0.000016540438,0.0007457153,0.000005832446],"about_ca_topic_score_codex":0.006157026,"about_ca_topic_score_gemma":0.015520884,"teacher_disagreement_score":0.006157026,"about_ca_system_score_codex":0.0003264252,"about_ca_system_score_gemma":0.00013995347,"threshold_uncertainty_score":0.012242377},"labels":[],"label_agreement":null},{"id":"W4385813470","doi":"10.3847/1538-4357/ace349","title":"The Role of Natal Kicks in Forming Asymmetric Compact Binary Mergers","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Gravitational wave; Neutron star; Compact star; Mass ratio; LIGO; Merge (version control); Binary number; Asymmetry; Binary black hole; Binary star; Population; Astronomy; Stellar mass; Stars; Star formation; Quantum mechanics","score_opus":0.010847461345658758,"score_gpt":0.31192439683897016,"score_spread":0.3010769354933114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385813470","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99802953,0.00007504386,0.0006084196,0.000062046165,0.0000042516294,0.0000052490154,0.000023427336,0.000020006019,0.0011718691],"genre_scores_gemma":[0.9997936,0.000017032695,0.00008526556,0.0000056479303,0.0000016732133,0.0000013528853,0.000012079198,0.000003790268,0.00007962243],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998276,0.000046819245,0.000012082169,0.000034321118,0.000026582607,0.000052539483],"domain_scores_gemma":[0.9982728,0.00062027,0.0004949791,0.0000818955,0.00008238706,0.00044774625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000632017,0.00031526282,0.00040469688,0.0007765157,0.0007566491,0.0015294738,0.00061775086,0.00063681515,0.002187732],"category_scores_gemma":[0.004036724,0.0003500788,0.00030254532,0.00026398426,0.00075857027,0.001405464,0.0013419061,0.0004511431,0.00027544738],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015706272,0.00040045625,0.6041981,0.00014716854,0.00034433728,0.002226229,0.0008127834,0.32266068,0.028777897,0.020143757,0.0009902786,0.017727578],"study_design_scores_gemma":[0.00015797162,0.00042603273,0.25313342,0.000043253734,0.00015399599,0.0008166858,0.00096389605,0.72566235,0.006614136,0.010474499,0.0014581343,0.000095702126],"about_ca_topic_score_codex":0.0027666036,"about_ca_topic_score_gemma":0.0025573217,"teacher_disagreement_score":0.0027666036,"about_ca_system_score_codex":0.0007183063,"about_ca_system_score_gemma":0.000304647,"threshold_uncertainty_score":0.0073186755},"labels":[],"label_agreement":null},{"id":"W4385813532","doi":"10.3847/1538-4357/ace1eb","title":"On the Tidal Capture of White Dwarfs by Intermediate-mass Black Holes in Dense Stellar Environments","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; White dwarf; Globular cluster; Supermassive black hole; Gravitational wave; Intermediate-mass black hole; Star cluster; Einstein Telescope; Black hole (networking); Star (game theory); Stars; Astronomy; Galaxy","score_opus":0.009158723675597391,"score_gpt":0.26924348725706715,"score_spread":0.26008476358146976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385813532","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99927706,0.00004454448,0.0002852779,0.000013902916,9.287912e-7,0.0000013818112,0.000011228568,0.0000026684331,0.00036299723],"genre_scores_gemma":[0.9998254,0.000022904993,0.00005009365,0.0000038851745,0.0000011321446,4.5742294e-7,0.000009626092,6.5356306e-7,0.00008594621],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999897,0.00001954855,0.000003452973,0.000021023436,0.000018682891,0.00004021332],"domain_scores_gemma":[0.999236,0.00026404805,0.00026042954,0.00008126178,0.000051045514,0.00010720705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004972789,0.00017415914,0.00018004586,0.00039199507,0.00032397563,0.00044010504,0.00029012654,0.00022383533,0.0010689283],"category_scores_gemma":[0.0010934116,0.00011324906,0.00014277901,0.00019912825,0.00061488524,0.00044725917,0.00054534886,0.00014684768,0.00017766938],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045894782,0.00013693768,0.92760485,0.00005929828,0.000101927,0.0005878287,0.0007459017,0.007865923,0.043433167,0.005656564,0.0003498824,0.012998854],"study_design_scores_gemma":[0.000022209053,0.00032379365,0.93440515,0.00001938653,0.000058202564,0.00037493455,0.0012681665,0.045772623,0.0129931485,0.0038928564,0.0008481837,0.000021260812],"about_ca_topic_score_codex":0.003578238,"about_ca_topic_score_gemma":0.0032407977,"teacher_disagreement_score":0.003578238,"about_ca_system_score_codex":0.00032630167,"about_ca_system_score_gemma":0.0001104218,"threshold_uncertainty_score":0.0071148276},"labels":[],"label_agreement":null},{"id":"W4385813538","doi":"10.3847/1538-4357/ace340","title":"Comparing Globular Cluster System Properties with Host Galaxy Environment*","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Impact of Light on Environment and Health","field":"Environmental Science","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Globular cluster; Astronomy; Brightest cluster galaxy; Metallicity; Type-cD galaxy; Galaxy; Elliptical galaxy; Photometry (optics); Galaxy cluster; Interacting galaxy; Stars","score_opus":0.019907908239384188,"score_gpt":0.20627424857107912,"score_spread":0.18636634033169494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385813538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99926513,0.00003137102,0.000044048174,0.000006796634,4.0174035e-7,0.0000013529378,0.00033039472,0.0000033723968,0.00031718164],"genre_scores_gemma":[0.9996346,0.00001008546,0.000022360873,0.0000021642445,8.2834595e-7,5.7578524e-7,0.00024633075,0.0000011697826,0.0000818544],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986684,0.0000188509,0.000007940292,0.00004385784,0.0000319829,0.00003047043],"domain_scores_gemma":[0.9991374,0.00017607996,0.00030231988,0.000072315815,0.00011736595,0.00019453434],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002487945,0.0001408659,0.00017355838,0.001002543,0.00020723617,0.00042800172,0.00016454984,0.00019267286,0.0026798153],"category_scores_gemma":[0.000986369,0.00006249278,0.00012472589,0.0007452385,0.00023223532,0.00018356917,0.00032465337,0.00009531225,0.00035244683],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000025417192,0.0000048226893,0.99836975,0.0000030691092,0.000020603246,0.000013316583,0.000030177562,0.0002203184,0.000674128,0.000020181422,0.000042209693,0.0005758753],"study_design_scores_gemma":[4.1384354e-7,0.000008799574,0.99959856,4.9921914e-7,0.0000037186683,0.000016579219,0.00002644008,0.00021046396,0.00007627677,0.000012790734,0.000044651886,7.3062324e-7],"about_ca_topic_score_codex":0.009647875,"about_ca_topic_score_gemma":0.012657426,"teacher_disagreement_score":0.009647875,"about_ca_system_score_codex":0.00024719868,"about_ca_system_score_gemma":0.00011428726,"threshold_uncertainty_score":0.019183457},"labels":[],"label_agreement":null},{"id":"W4385813772","doi":"10.3847/1538-4357/acd546","title":"Morphological Parameters and Associated Uncertainties for 8 Million Galaxies in the Hyper Suprime-Cam Wide Survey","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Mila - Quebec Artificial Intelligence Institute","funders":"Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Fondo Nacional de Desarrollo Científico y Tecnológico; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Bulge; Stars; Bayesian probability; RADIUS; Galaxy formation and evolution; Spitzer Space Telescope; Effective radius; Algorithm; Artificial intelligence; Computer science","score_opus":0.025306155071626,"score_gpt":0.2418389967576017,"score_spread":0.2165328416859757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385813772","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9820525,0.0003228254,0.007617818,0.00017682134,0.000010881597,0.00001837127,0.006549548,0.0005668458,0.0026843797],"genre_scores_gemma":[0.97779715,0.00009873737,0.007500602,0.00004819589,0.00001655726,0.0000330035,0.013946761,0.000054472235,0.0005045068],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994623,0.000180983,0.00003219767,0.00013502566,0.00015119014,0.000038325554],"domain_scores_gemma":[0.9977704,0.00071572827,0.00049669895,0.00055031397,0.00033977607,0.00012698726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021486895,0.00040984282,0.00028078648,0.0019455631,0.00028607433,0.00061343884,0.00077094714,0.0004247884,0.0013599058],"category_scores_gemma":[0.005659264,0.000256978,0.00051911926,0.0013503426,0.0002979576,0.00040029557,0.0010491367,0.0003859067,0.0005675439],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023069605,0.000043072632,0.87897104,0.000051319224,0.00022298135,0.00011973296,0.00015895734,0.067160144,0.0024302874,0.0016987042,0.0047032377,0.044209808],"study_design_scores_gemma":[0.00003939846,0.000038110153,0.84748465,0.000048453032,0.00004806648,0.000101933605,0.000118956144,0.14224546,0.0026450297,0.0017405147,0.0054511745,0.000038297967],"about_ca_topic_score_codex":0.019953461,"about_ca_topic_score_gemma":0.022888748,"teacher_disagreement_score":0.019953461,"about_ca_system_score_codex":0.000747698,"about_ca_system_score_gemma":0.00023993815,"threshold_uncertainty_score":0.03967464},"labels":[],"label_agreement":null},{"id":"W4385879722","doi":"10.3847/1538-4357/ace421","title":"On the Proposed Interstellar Origin of the USG 20140108 Fireball","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Grantová Agentura České Republiky; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Drag; Astronomy; Mechanics","score_opus":0.013919839382348528,"score_gpt":0.2208169079861349,"score_spread":0.20689706860378637,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385879722","genre_codex":"review","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.3097603,0.509445,0.006563993,0.013162514,0.005438099,0.0001648286,0.0010093448,0.0003048863,0.15415111],"genre_scores_gemma":[0.7447276,0.22011542,0.0044066575,0.006153634,0.00391831,0.000054785964,0.00157663,0.0000657934,0.018981084],"study_design_codex":"design_other","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99978036,0.000019089546,0.000019485817,0.000059385922,0.000081910766,0.000039822397],"domain_scores_gemma":[0.99940884,0.00015317551,0.0001329759,0.000033080432,0.00022902036,0.000043007974],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009861384,0.0007373049,0.00035791626,0.0026034887,0.0008839037,0.0017414122,0.0007597948,0.0009014377,0.002830704],"category_scores_gemma":[0.0009798411,0.00020686816,0.00038262986,0.001258993,0.0012026363,0.0009841889,0.00079921033,0.0010423413,0.0008522365],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010142747,0.00013310557,0.07939506,0.005398892,0.00047334816,0.01142382,0.0009535624,0.003186642,0.03789092,0.06327002,0.03732136,0.75953907],"study_design_scores_gemma":[0.000050663097,0.0005772503,0.21284588,0.0047460366,0.00031576504,0.0062720138,0.0021552152,0.0016644116,0.013042947,0.025220811,0.7330197,0.00008929899],"about_ca_topic_score_codex":0.008165145,"about_ca_topic_score_gemma":0.006224265,"teacher_disagreement_score":0.008165145,"about_ca_system_score_codex":0.0018621873,"about_ca_system_score_gemma":0.0010366752,"threshold_uncertainty_score":0.016235232},"labels":[],"label_agreement":null},{"id":"W4385880428","doi":"10.3847/1538-4357/acdc1b","title":"Search for sub-TeV Neutrino Emission from Novae with IceCube-DeepCore","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Alberta","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; National Research Foundation; Michigan State University; University of Oxford; Chiba University; Santen; Compute Canada; Marquette University","keywords":"Physics; Neutrino; Astrophysics; Luminosity; White dwarf; Neutrino astronomy; Astronomy; Nova (rocket); Fermi Gamma-ray Space Telescope; Observatory; Solar neutrino problem; Neutrino detector; Stars; Solar neutrino; Neutrino oscillation; Nuclear physics; Galaxy","score_opus":0.016431665109643785,"score_gpt":0.24766947108241555,"score_spread":0.23123780597277177,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385880428","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97744,0.0006132336,0.0021968647,0.000106909596,0.000036205754,0.0000913079,0.013012015,0.0002482548,0.0062551764],"genre_scores_gemma":[0.95548296,0.0003508753,0.011423647,0.00023667376,0.000055449866,0.00008879567,0.031063357,0.00009947527,0.0011987966],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99957234,0.000047657115,0.00001553629,0.00012316975,0.00014982461,0.0000915677],"domain_scores_gemma":[0.99891067,0.00021824453,0.00038216854,0.00014125826,0.0001276335,0.00022006976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00092830573,0.00046735632,0.00043474176,0.0014596205,0.00042419237,0.000730949,0.00047341725,0.00043897587,0.0016712061],"category_scores_gemma":[0.0009980348,0.00025948312,0.00043751474,0.0012509795,0.0002935838,0.00036719255,0.0011502359,0.00038705656,0.00037831697],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012076015,0.0002088052,0.893483,0.00013944064,0.0003653639,0.0006743253,0.00024781408,0.0023619574,0.07759431,0.00077600003,0.0044130646,0.018528175],"study_design_scores_gemma":[0.00008287756,0.0002827969,0.9436697,0.00004419803,0.000141664,0.0010601277,0.00026702555,0.006448943,0.024890667,0.00056622655,0.022516806,0.000028927012],"about_ca_topic_score_codex":0.0044016484,"about_ca_topic_score_gemma":0.011663681,"teacher_disagreement_score":0.0044016484,"about_ca_system_score_codex":0.00046827362,"about_ca_system_score_gemma":0.00034347433,"threshold_uncertainty_score":0.008752048},"labels":[],"label_agreement":null},{"id":"W4385950984","doi":"10.3847/1538-4357/ace2c4","title":"Investigating the Origin of the Absorption-line Variability in the Narrow-line Seyfert 1 Galaxy WPVS 007","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Western University","funders":"Natural Sciences and Engineering Research Council of Canada; Supercomputing Center for Education and Research, University of Oklahoma; Goddard Space Flight Center; Compute Canada; University of Oklahoma; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Quasar; Astrophysics; Outflow; Physics; Supermassive black hole; Galaxy; Redshift; Spectral line; Absorption (acoustics); Luminosity; Absorption spectroscopy; Astronomy; Optics; Meteorology","score_opus":0.01907288150953756,"score_gpt":0.25078782671391936,"score_spread":0.2317149452043818,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385950984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995447,0.000013435373,0.0001934715,0.00000502195,6.663718e-7,0.0000010134246,0.0000835891,0.000013531157,0.00014450532],"genre_scores_gemma":[0.999634,0.000006252217,0.00018058717,0.000002484386,0.0000012847197,0.0000013430329,0.00013550556,0.0000055596706,0.000032849184],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993384,0.000010289624,0.0000026543569,0.000027619835,0.000011229756,0.000014438143],"domain_scores_gemma":[0.99963427,0.00010490141,0.00011429513,0.000043432083,0.00003165153,0.00007144444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025840744,0.00014723874,0.00015543983,0.0008047351,0.00015101358,0.00040557957,0.00022708601,0.00017766752,0.000504993],"category_scores_gemma":[0.00052751234,0.000109905595,0.00020657468,0.00033185075,0.00026898092,0.0002482365,0.00030006116,0.00015307104,0.00010333953],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012903952,0.00006405415,0.9323079,0.000029008414,0.0000933637,0.000200235,0.00034332927,0.0052964683,0.051828664,0.00063004036,0.0002482652,0.00882959],"study_design_scores_gemma":[0.000007205754,0.00004096624,0.9770521,0.000003930207,0.000018246761,0.000051736864,0.0001292326,0.020362347,0.0018983766,0.00019701823,0.00023287129,0.000006016053],"about_ca_topic_score_codex":0.003651357,"about_ca_topic_score_gemma":0.004794546,"teacher_disagreement_score":0.003651357,"about_ca_system_score_codex":0.00032841298,"about_ca_system_score_gemma":0.000092450835,"threshold_uncertainty_score":0.0072602034},"labels":[],"label_agreement":null},{"id":"W4385971196","doi":"10.3847/1538-4357/acdd5e","title":"Hard X-Ray Observation and Multiwavelength Study of the PeVatron Candidate Pulsar Wind Nebula “Dragonfly”","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"National Aeronautics and Space Administration","keywords":"Physics; Nebula; Astrophysics; Pulsar wind nebula; Pulsar; Astronomy; Stars","score_opus":0.021773541438671752,"score_gpt":0.3089798327074723,"score_spread":0.28720629126880054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4385971196","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99905235,0.000044161225,0.00012071332,0.000013576751,0.000002117817,0.000004613877,0.00012395163,0.00000837168,0.00063016854],"genre_scores_gemma":[0.9985159,0.000029854255,0.00046840144,0.00002406455,0.0000057088146,0.000005640341,0.000515093,0.000005136299,0.0004301857],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994636,0.000003830521,0.0000015624978,0.00002064222,0.000011605924,0.000016064743],"domain_scores_gemma":[0.99986255,0.00001686901,0.000030410787,0.000016984784,0.000015480862,0.000057723624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001344577,0.00021923543,0.00015564302,0.00066700194,0.00050023716,0.0003123483,0.00021751164,0.00019401935,0.0006462045],"category_scores_gemma":[0.00013889627,0.00012900232,0.00012589402,0.00027130925,0.00018840363,0.00016368306,0.00037606063,0.0002334221,0.0001222226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043188033,0.00020057675,0.74634945,0.000047592246,0.0001016142,0.0028023021,0.000655604,0.0006670937,0.22876695,0.00039461793,0.0012150684,0.018367266],"study_design_scores_gemma":[0.0000071898585,0.000083746345,0.993903,0.0000038052256,0.000011193483,0.00041507767,0.00009619869,0.00047969248,0.0035689664,0.00003177804,0.0013943753,0.000004920595],"about_ca_topic_score_codex":0.0030051386,"about_ca_topic_score_gemma":0.009885295,"teacher_disagreement_score":0.0030051386,"about_ca_system_score_codex":0.00027514214,"about_ca_system_score_gemma":0.000092412854,"threshold_uncertainty_score":0.005975306},"labels":[],"label_agreement":null},{"id":"W4386043538","doi":"10.3847/1538-4357/acf49d","title":"Atmospheric Effects on Neutron Star Parameter Constraints with NICER","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"HORIZON EUROPE European Research Council; China Scholarship Council; Nuclear Safety and Security Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Centre National d’Etudes Spatiales; Natural Sciences and Engineering Research Council of Canada; European Commission; National Aeronautics and Space Administration","keywords":"Physics; Millisecond pulsar; RADIUS; Ionization; Astrophysics; Helium; Neutron star; Pulsar; Atmosphere (unit); Hydrogen; Astronomy; Atomic physics","score_opus":0.009509333394431902,"score_gpt":0.289701070992401,"score_spread":0.2801917375979691,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386043538","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9847839,0.00072926906,0.0075812354,0.0002580026,0.000019726576,0.000012958787,0.0015623859,0.00063285744,0.0044196798],"genre_scores_gemma":[0.9940798,0.0000741099,0.0036786932,0.00006196704,0.000020786272,0.000008079324,0.0017721428,0.00014937184,0.00015509478],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99489355,0.0023452016,0.00026819014,0.0011754826,0.0010017512,0.00031586603],"domain_scores_gemma":[0.97555417,0.013977145,0.003830744,0.0046808133,0.0015314014,0.00042570804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.008801711,0.0003970164,0.0007555111,0.000861714,0.00041876634,0.0012570346,0.001470135,0.0005804462,0.0011335226],"category_scores_gemma":[0.02239668,0.00036678376,0.0013084218,0.00082504173,0.00059413584,0.0011345737,0.00168529,0.0006722477,0.00033962558],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015303998,0.000071388095,0.6761998,0.00030410057,0.0015156196,0.0006058551,0.00048577198,0.262943,0.016125374,0.005310119,0.0028824615,0.03202621],"study_design_scores_gemma":[0.00014096733,0.00031890045,0.57063884,0.000109819084,0.00054042164,0.0007823598,0.00022683282,0.39734468,0.014318035,0.0025190993,0.012871911,0.00018809442],"about_ca_topic_score_codex":0.005479955,"about_ca_topic_score_gemma":0.004411108,"teacher_disagreement_score":0.008801711,"about_ca_system_score_codex":0.0011263057,"about_ca_system_score_gemma":0.00035138702,"threshold_uncertainty_score":0.046548486},"labels":[],"label_agreement":null},{"id":"W4386072606","doi":"10.3847/1538-4357/ace43c","title":"The Imprint of Convection on Type I X-Ray Bursts: Pauses in Photospheric Radius Expansion Lightcurves","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; McGill University Health Centre","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Convection; Neutron star; RADIUS; Luminosity; Mixing (physics); Envelope (radar); Astronomy; Mechanics","score_opus":0.014977626301788189,"score_gpt":0.246512795053804,"score_spread":0.2315351687520158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386072606","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99792874,0.000048921334,0.00077932543,0.00003932402,0.0000056608037,0.000005190184,0.0001673115,0.00012266035,0.000902757],"genre_scores_gemma":[0.9994904,0.0000127528365,0.00024210868,0.0000045206707,0.0000021637672,0.000003312277,0.00011000255,0.000028017641,0.00010671792],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99993086,0.000016327062,0.0000040075115,0.00001624648,0.000013238082,0.000019264418],"domain_scores_gemma":[0.9995185,0.00021345376,0.00009649471,0.000054999702,0.00003170015,0.000084867344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027607288,0.00034436054,0.00023227386,0.00027141973,0.00022538388,0.00054813403,0.0003891215,0.00039312278,0.0014497469],"category_scores_gemma":[0.0009968873,0.00016310255,0.00043918204,0.00020427752,0.00040935102,0.00025363814,0.00042805888,0.00047021333,0.0001284605],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013245904,0.0003404634,0.3245343,0.00011027295,0.00021067006,0.00082110695,0.0004650619,0.5768385,0.07908059,0.002799279,0.0011073141,0.012367872],"study_design_scores_gemma":[0.00008918912,0.0002694252,0.28927806,0.000023805493,0.00003600629,0.00012926792,0.0001594788,0.6938801,0.014372848,0.0007952813,0.00093122444,0.00003532704],"about_ca_topic_score_codex":0.0033824844,"about_ca_topic_score_gemma":0.0021101607,"teacher_disagreement_score":0.0033824844,"about_ca_system_score_codex":0.0004373515,"about_ca_system_score_gemma":0.00012903653,"threshold_uncertainty_score":0.0067255497},"labels":[],"label_agreement":null},{"id":"W4386072634","doi":"10.3847/1538-4357/ace042","title":"An Unsupervised Machine Learning-based Algorithm for Detecting Weak Impulsive Narrowband Quiet Sun Emissions and Characterizing Their Morphology","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"National Science Foundation","keywords":"Physics; Narrowband; Nanoflares; QUIET; Coronal hole; Solar wind; Astrophysics; Algorithm; Coronal mass ejection; Corona (planetary geology); Astronomy; Computer science; Plasma; Optics","score_opus":0.009985472751859644,"score_gpt":0.24696081960850458,"score_spread":0.23697534685664493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386072634","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.094977014,0.00039775157,0.89862686,0.0004160031,0.000085003376,0.00022648402,0.0002917891,0.0037447743,0.0012342292],"genre_scores_gemma":[0.41717726,0.00012510041,0.57819027,0.00039395146,0.00010918416,0.0004768104,0.0013443574,0.00013229832,0.0020507628],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99900407,0.0001673682,0.00010230047,0.00036586678,0.00022688865,0.00013358908],"domain_scores_gemma":[0.9979177,0.00101757,0.00024548642,0.00017263694,0.0005370104,0.00010959875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017309792,0.0010145787,0.0012425754,0.0020977596,0.00082075526,0.0012565312,0.0025157342,0.002315861,0.0014712533],"category_scores_gemma":[0.004555197,0.00043346928,0.001026037,0.0015160549,0.00071294216,0.0008864103,0.0009683509,0.0014805053,0.0009179421],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043307012,0.00056401145,0.014106293,0.00013873304,0.00020752107,0.00023071501,0.00011757301,0.29360715,0.01753926,0.0027195956,0.0052744923,0.6650616],"study_design_scores_gemma":[0.000015652142,0.00003356905,0.0007655753,0.000005097966,0.000007783693,0.00002462895,0.000012850395,0.9964677,0.0013154771,0.0010949312,0.00025013112,0.0000066422326],"about_ca_topic_score_codex":0.005189499,"about_ca_topic_score_gemma":0.0044534905,"teacher_disagreement_score":0.005189499,"about_ca_system_score_codex":0.00097502104,"about_ca_system_score_gemma":0.0015039179,"threshold_uncertainty_score":0.010318577},"labels":[],"label_agreement":null},{"id":"W4386082869","doi":"10.3847/1538-4357/ace595","title":"SN 2020bio: A Double-peaked, H-poor Type IIb Supernova with Evidence of Circumstellar Interaction","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Horizon 2020 Framework Programme; Israel Science Foundation; National Aeronautics and Space Administration; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Supernova; Astrophysics; Light curve; RADIUS; Luminosity; Type (biology); Astronomy; Galaxy","score_opus":0.03280430816472953,"score_gpt":0.27837819063428376,"score_spread":0.24557388246955422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386082869","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99619484,0.00021024757,0.00041352754,0.000024319244,0.000020093872,0.000015852613,0.0003404861,0.00002841183,0.0027522584],"genre_scores_gemma":[0.9981184,0.00006983895,0.0004249286,0.00006206033,0.000022486603,0.0000061193773,0.000758322,0.000006796997,0.00053107215],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999403,0.000003858649,0.0000045254374,0.000018546896,0.000015859674,0.000016940743],"domain_scores_gemma":[0.9997874,0.000013181009,0.00004466083,0.00001412749,0.000017011436,0.00012356737],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013550128,0.0006085757,0.00032068786,0.0005574854,0.0003821438,0.00041326333,0.00024472582,0.0004167999,0.0014303066],"category_scores_gemma":[0.00017102878,0.00017768635,0.0002150548,0.00027658293,0.00022354166,0.00013497603,0.00044343653,0.00029591535,0.00039061357],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013947207,0.00030390316,0.79778314,0.000099129684,0.00017308583,0.0170546,0.0001340497,0.0006294624,0.16626571,0.000915061,0.0018558026,0.0133913485],"study_design_scores_gemma":[0.000039881925,0.00056859764,0.9523265,0.000021257176,0.000034717355,0.030799758,0.00018704915,0.0017032742,0.008487931,0.00034943598,0.005467235,0.000014375426],"about_ca_topic_score_codex":0.001600494,"about_ca_topic_score_gemma":0.0025715993,"teacher_disagreement_score":0.001600494,"about_ca_system_score_codex":0.0001866736,"about_ca_system_score_gemma":0.00010468404,"threshold_uncertainty_score":0.0047848225},"labels":[],"label_agreement":null},{"id":"W4386099907","doi":"10.3847/1538-4357/ace596","title":"The Long-term Spectral Changes of Eta Carinae: Are they Caused by a Dissipating Occulter as Indicated by cmfgen Models?","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Astrophysics; Light curve; Luminosity; Brightness; Emission spectrum; Spectral line; Line (geometry); Effective temperature; Astronomy; Line-of-sight; Stars; Galaxy","score_opus":0.017941969745415443,"score_gpt":0.251327252640793,"score_spread":0.23338528289537752,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386099907","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913838,0.00042762817,0.0026877322,0.00041439832,0.000029320228,0.000010821392,0.00017378743,0.00008849443,0.0047839913],"genre_scores_gemma":[0.99931526,0.000042898104,0.00018080941,0.000018708115,0.0000075606654,0.0000031524455,0.000051537507,0.000017927518,0.0003622546],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998698,0.000024175164,0.000006150599,0.000049164337,0.000017999568,0.000032659125],"domain_scores_gemma":[0.99962306,0.000068497975,0.0000982188,0.00006328408,0.000054729957,0.0000922595],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033622503,0.0004952845,0.00030112866,0.0005730942,0.000449601,0.0008118593,0.0010324267,0.0008608166,0.002504702],"category_scores_gemma":[0.0009081487,0.00021522053,0.00063602,0.00027086883,0.0005337084,0.0007431878,0.000512244,0.00036974292,0.00047045472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00088820443,0.00025361174,0.59823537,0.00021828948,0.00046249316,0.0026834514,0.0011009807,0.30940208,0.03821727,0.017561704,0.0028591957,0.028117476],"study_design_scores_gemma":[0.000048322934,0.00011275865,0.25673544,0.00003240284,0.00012443545,0.0005274401,0.00034215234,0.73170125,0.0024482508,0.0044005793,0.0034703552,0.000056656023],"about_ca_topic_score_codex":0.008641613,"about_ca_topic_score_gemma":0.00394515,"teacher_disagreement_score":0.008641613,"about_ca_system_score_codex":0.0009973723,"about_ca_system_score_gemma":0.00017343811,"threshold_uncertainty_score":0.017182589},"labels":[],"label_agreement":null},{"id":"W4386100204","doi":"10.3847/1538-4357/acdfcb","title":"Search for Correlations of High-energy Neutrinos Detected in IceCube with Radio-bright AGN and Gamma-Ray Emission from Blazars","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; National Research Foundation; Michigan State University; University of Oxford; Chiba University; Santen; Compute Canada; Marquette University","keywords":"Physics; Blazar; Neutrino; Astrophysics; Fermi Gamma-ray Space Telescope; Active galactic nucleus; Gamma ray; Observatory; Astronomy; Astroparticle physics; Galaxy; Particle physics","score_opus":0.00858519662662307,"score_gpt":0.21614636443191604,"score_spread":0.20756116780529296,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386100204","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964804,0.00006773625,0.00060894474,0.000021068072,0.000005339003,0.00001643287,0.0015107373,0.0000340236,0.0012553607],"genre_scores_gemma":[0.99377173,0.000049449733,0.0013976352,0.000020389203,0.00001642563,0.000023943954,0.0043216157,0.000017724604,0.00038112234],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993666,0.00015703897,0.00006232868,0.00017879222,0.0001496594,0.000085660526],"domain_scores_gemma":[0.9946733,0.0025370975,0.0016396674,0.00044049392,0.0003751112,0.00033426587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010058676,0.00025021157,0.00030344576,0.0026861222,0.0003060668,0.0010619446,0.00026254778,0.00025566274,0.0029645283],"category_scores_gemma":[0.003433521,0.00013339432,0.00027325572,0.0021490841,0.00024340478,0.0003978727,0.0005258572,0.0003271333,0.00040277137],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011268333,0.000025328001,0.9955449,0.000007941706,0.0000805055,0.00007085896,0.000038411035,0.00016686154,0.0018531563,0.00006878918,0.00018987343,0.0018405562],"study_design_scores_gemma":[0.0000105178315,0.000056382494,0.99550986,0.000005853591,0.000050296872,0.00021536359,0.00011675084,0.0016314792,0.0017432477,0.000063976986,0.0005921533,0.0000040296],"about_ca_topic_score_codex":0.00368714,"about_ca_topic_score_gemma":0.0047921324,"teacher_disagreement_score":0.00368714,"about_ca_system_score_codex":0.0002569077,"about_ca_system_score_gemma":0.00045830067,"threshold_uncertainty_score":0.009917319},"labels":[],"label_agreement":null},{"id":"W4386114804","doi":"10.3847/1538-4357/ace695","title":"Alignments between Galaxies and the Cosmic Web at z ∼ 1–2 in the IllustrisTNG Simulations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Lawrence Berkeley National Laboratory; Ministry of Education, Culture, Sports, Science and Technology; Office of Science; Japan Society for the Promotion of Science; Yukawa Institute for Theoretical Physics, Kyoto University; National Energy Research Scientific Computing Center","keywords":"Physics; Galaxy; Redshift; Cosmic variance; Astrophysics; COSMIC cancer database; SIGNAL (programming language); Galaxy formation and evolution; Weak gravitational lensing; Bispectrum; Statistics; Computer science","score_opus":0.013604963641974782,"score_gpt":0.23546550789499723,"score_spread":0.22186054425302246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386114804","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981488,0.0000129454465,0.00031400757,0.000070040915,0.000004452986,0.0000051468833,0.00035010837,0.00006213489,0.0010324485],"genre_scores_gemma":[0.99813795,0.0000110799,0.000710298,0.000035916957,0.0000049421606,0.000008137303,0.00089218747,0.00002698324,0.00017238052],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986124,0.00003211482,0.0000072101093,0.000034015247,0.00002096906,0.000044535802],"domain_scores_gemma":[0.9990337,0.00037030625,0.00014144609,0.00012257129,0.000092298615,0.00023964058],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00045455308,0.00032956497,0.00037062343,0.00039596454,0.00041100878,0.00067677326,0.0008339786,0.0005804166,0.0014737984],"category_scores_gemma":[0.0023955638,0.00025318147,0.0005663006,0.0003550854,0.00060216954,0.0003584421,0.0006054349,0.00063742016,0.000112327354],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004507928,0.00025467403,0.23571537,0.00005097178,0.00023676551,0.0002862424,0.00023103855,0.7459337,0.0065969215,0.0047760876,0.0018374884,0.003629847],"study_design_scores_gemma":[0.0001378484,0.00018480684,0.09715281,0.000015498734,0.00006661184,0.000066865796,0.00013930633,0.8975992,0.0026527524,0.0011893569,0.000754854,0.00004002995],"about_ca_topic_score_codex":0.025143972,"about_ca_topic_score_gemma":0.022437265,"teacher_disagreement_score":0.025143972,"about_ca_system_score_codex":0.00076489244,"about_ca_system_score_gemma":0.0004390359,"threshold_uncertainty_score":0.049995244},"labels":[],"label_agreement":null},{"id":"W4386121105","doi":"10.3847/1538-4357/ace969","title":"NuSTAR Observations of Abell 665 and 2146: Constraints on Nonthermal Emission","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"NASA Headquarters","keywords":"Physics; Astrophysics; Astronomy; Thermal emission; Thermal; Meteorology","score_opus":0.02513099578346376,"score_gpt":0.24804033497430766,"score_spread":0.2229093391908439,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386121105","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999081,0.00006704198,0.00021148442,0.000009975351,0.0000016805159,0.0000016310797,0.000130299,0.000014997242,0.00048183397],"genre_scores_gemma":[0.9991448,0.000024955089,0.00025742277,0.000008306673,0.000002294127,0.000001388934,0.00038274418,0.000004750238,0.00017333915],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998516,0.000017263883,0.0000131710985,0.000041710944,0.000044848897,0.000031420223],"domain_scores_gemma":[0.9995679,0.000040447085,0.00016788082,0.000054258137,0.000040844556,0.00012859047],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002781781,0.00034567146,0.00035190076,0.0006713306,0.000451073,0.0005789657,0.00025239118,0.00032900996,0.0009686453],"category_scores_gemma":[0.0004989925,0.00019592245,0.0004479702,0.0005285869,0.00028632183,0.00020565493,0.000493009,0.00018126058,0.00036159178],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041559053,0.00005760949,0.92736286,0.000061694074,0.0001260148,0.00024218303,0.00028917816,0.0067861606,0.05901354,0.00049992406,0.00027715496,0.00486802],"study_design_scores_gemma":[0.000013927408,0.000081941056,0.98824906,0.000008495332,0.0000356875,0.00013167626,0.0001323907,0.0069055143,0.0035857686,0.00013967519,0.0007066048,0.000009234674],"about_ca_topic_score_codex":0.006231923,"about_ca_topic_score_gemma":0.01195916,"teacher_disagreement_score":0.006231923,"about_ca_system_score_codex":0.00038374442,"about_ca_system_score_gemma":0.00015618237,"threshold_uncertainty_score":0.012391329},"labels":[],"label_agreement":null},{"id":"W4386121218","doi":"10.3847/1538-4357/ace5aa","title":"The Demographics, Stellar Populations, and Star Formation Histories of Fast Radio Burst Host Galaxies: Implications for the Progenitors","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":113,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"SLAC National Accelerator Laboratory; Los Alamos National Laboratory; Argonne National Laboratory; Planetary Science Division; Australian Research Council; Quest High Performance Computing; Science Mission Directorate; College of Engineering, Michigan State University; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; Office of Science; University of Illinois at Urbana-Champaign; Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Commonwealth Scientific and Industrial Research Organisation; Eötvös Loránd Tudományegyetem; Brookhaven National Laboratory; Max-Planck-Gesellschaft; Science and Technology Facilities Council; York University; Ministério da Ciência, Tecnologia e Inovação; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Deutsche Forschungsgemeinschaft; European Southern Observatory; National Central University; Space Telescope Science Institute; University of Sussex; European Commission; Gordon and Betty Moore Foundation; Australian Government; Princeton University; NASA Exoplanet Science Institute; Korea Astronomy and Space Science Institute; National Astronomical Observatory of Japan; University of Portsmouth; New Mexico State University; Smithsonian Astrophysical Observatory; European Space Agency; University of California, Los Angeles; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Mellon University; Fermilab; Max-Planck-Institut für Astronomie; Michigan State University; Vanderbilt University; University of Chicago; Integrated Electronics Engineering Center, Binghamton University; Queen's University; University of North Carolina at Chapel Hill; Harvard University; Durham University; Northwestern University; Ohio State University; Research Corporation for Science Advancement; Government of Western Australia; Yale University; U.S. Department of Energy; Smithsonian Institution; Financiadora de Estudos e Projetos; University of Pennsylvania; University College London; National Aeronautics and Space Administration; Science and Industry Endowment Fund; Queen's University Belfast; Macquarie University; W. M. Keck Foundation; California Institute of Technology; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Stellar mass; Stellar population; Supernova; Astronomy; Population; Magnetar; Stellar evolution; Stars; Neutron star; Medicine","score_opus":0.023880205502404377,"score_gpt":0.3168130554661736,"score_spread":0.2929328499637692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386121218","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991671,0.00016777606,0.000201722,0.000030923475,7.0605677e-7,0.0000020251362,0.00024076673,0.0000038535773,0.00018508967],"genre_scores_gemma":[0.99953413,0.00008450886,0.000109574205,0.000006326238,0.0000028460822,0.0000015791856,0.00019786638,0.000002578064,0.000060694678],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997949,0.000054573404,0.000019931618,0.00006729597,0.00003335824,0.000029943425],"domain_scores_gemma":[0.9966834,0.0011067612,0.0013349043,0.0002462901,0.00015697743,0.0004717421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008641989,0.00021364643,0.00024551715,0.00082774943,0.00028559525,0.00095873384,0.00041338446,0.0002758382,0.0014096173],"category_scores_gemma":[0.004532348,0.00017208947,0.00023899633,0.00059227936,0.0003245429,0.0007280109,0.0004834526,0.00023729386,0.0003271455],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000014995308,0.0000041627163,0.9980742,0.0000026996586,0.000007716105,0.000018137005,0.000056006258,0.000101581405,0.00038453593,0.000034524237,0.0000197549,0.0012816441],"study_design_scores_gemma":[7.616177e-7,0.000018657733,0.9989849,0.0000032691469,0.000005514168,0.00009139413,0.00012851229,0.00051669433,0.00008895709,0.000083093255,0.00007655238,0.0000016862134],"about_ca_topic_score_codex":0.0034926794,"about_ca_topic_score_gemma":0.0032785954,"teacher_disagreement_score":0.0034926794,"about_ca_system_score_codex":0.00019490157,"about_ca_system_score_gemma":0.00018657873,"threshold_uncertainty_score":0.006944716},"labels":[],"label_agreement":null},{"id":"W4386160655","doi":"10.3847/1538-4357/acd77d","title":"Waltzing Binaries: Probing the Line-of-sight Acceleration of Merging Compact Objects with Gravitational Waves","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Department of Atomic Energy, Government of India","keywords":"Physics; Neutron star; Gravitational wave; Astrophysics; LIGO; Astronomy; Acceleration; Binary number; Context (archaeology); Line-of-sight; Supermassive black hole; Galaxy","score_opus":0.023839617964790085,"score_gpt":0.32095885317458783,"score_spread":0.29711923520979777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386160655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977502,0.00008340171,0.0007937316,0.000019353576,0.0000025552338,0.000009808412,0.00018379385,0.000032660297,0.0011244777],"genre_scores_gemma":[0.9984907,0.00002651541,0.0011281861,0.000012841018,0.0000053879085,0.000004194059,0.00021153451,0.000005420527,0.00011530232],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998685,0.000021145128,0.0000043128102,0.000035836194,0.00002701044,0.000043082822],"domain_scores_gemma":[0.9993259,0.0001418322,0.00025183446,0.00006152159,0.000054321412,0.00016459008],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005412272,0.00019904776,0.00025017912,0.0010528072,0.00031848619,0.0006732505,0.00024714522,0.0002928402,0.0011147695],"category_scores_gemma":[0.0008928815,0.00017163945,0.00013858076,0.0009079419,0.00022094717,0.00040421222,0.0007509385,0.0003191318,0.00023120028],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053775084,0.00013421538,0.92594725,0.000032465505,0.00012828509,0.00021962832,0.0002481193,0.0015150921,0.05661733,0.000979395,0.00029339668,0.013347004],"study_design_scores_gemma":[0.000025871865,0.00016387364,0.9841919,0.000007844202,0.000045404453,0.00016988919,0.00013487965,0.009338384,0.0047299042,0.00064447476,0.00053289114,0.00001466428],"about_ca_topic_score_codex":0.0023263763,"about_ca_topic_score_gemma":0.005655718,"teacher_disagreement_score":0.0023263763,"about_ca_system_score_codex":0.00025073814,"about_ca_system_score_gemma":0.000119965225,"threshold_uncertainty_score":0.004625678},"labels":[],"label_agreement":null},{"id":"W4386168895","doi":"10.3847/1538-4357/aced05","title":"IXPE and XMM-Newton Observations of the Soft Gamma Repeater SGR 1806–20","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Agenzia Spaziale Italiana; Istituto Nazionale di Fisica Nucleare; Canadian Space Agency; Nuclear Safety and Security Commission; Istituto Nazionale di Astrofisica; Japan Society for the Promotion of Science; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Magnetar; Astrophysics; Pulsar","score_opus":0.02583385038304304,"score_gpt":0.3080754407834781,"score_spread":0.28224159040043506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386168895","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961414,0.000106954765,0.00028911405,0.00004420215,0.000009990805,0.000013294085,0.00054925453,0.000053344873,0.0027925018],"genre_scores_gemma":[0.99321824,0.000114625676,0.0015350436,0.00007486614,0.000043030897,0.000020776872,0.0034316387,0.000038549806,0.0015233585],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998716,0.000011993692,0.000008688537,0.000036931404,0.000047306672,0.000023484297],"domain_scores_gemma":[0.9996269,0.000026467345,0.00014316698,0.000045180324,0.000051164043,0.00010720001],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027784574,0.00027704664,0.00023955802,0.0010159406,0.00027984282,0.0003964767,0.00018777861,0.00030307568,0.00096551445],"category_scores_gemma":[0.0004016895,0.00014667696,0.00021703228,0.00043305152,0.00021779494,0.00031280183,0.00091873185,0.00033010173,0.0005393511],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014252595,0.00030392793,0.5978491,0.00009040302,0.00016276547,0.0014085111,0.000771666,0.00069495634,0.35483798,0.00063941977,0.002374564,0.039441533],"study_design_scores_gemma":[0.000029367833,0.00017634367,0.98902786,0.0000055354035,0.00001784735,0.00048445768,0.00007988991,0.00035476856,0.0066234823,0.000074841206,0.003118702,0.000006769621],"about_ca_topic_score_codex":0.0007579423,"about_ca_topic_score_gemma":0.0013035883,"teacher_disagreement_score":0.0010159406,"about_ca_system_score_codex":0.00018114569,"about_ca_system_score_gemma":0.000081928156,"threshold_uncertainty_score":0.003229916},"labels":[],"label_agreement":null},{"id":"W4386169295","doi":"10.3847/1538-4357/acdcf9","title":"Eta Carinae: The Dissipating Occulter Is an Extended Structure","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; Goddard Space Flight Center; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Space Telescope Science Institute; Fundação de Amparo à Pesquisa do Estado de São Paulo; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Space Telescope Imaging Spectrograph; Astronomy; Spectrograph; Brightness; Ejecta; Spectral line; Radiation; Stars; Hubble space telescope; Supernova; Optics","score_opus":0.017333718135417005,"score_gpt":0.2781820477199322,"score_spread":0.2608483295845152,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386169295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99713886,0.000245686,0.00019452367,0.000052910887,0.00000773807,0.0000038962526,0.00007526876,0.000013492294,0.002267688],"genre_scores_gemma":[0.99879116,0.00005156582,0.0002196388,0.000022439079,0.000008158275,0.0000012449302,0.00012948942,0.000003428951,0.0007728657],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991465,0.000005664517,0.000004009193,0.000038741415,0.00001805792,0.000018906176],"domain_scores_gemma":[0.9997522,0.00001830814,0.000088511304,0.000030229612,0.000029970286,0.000080748556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010729441,0.00014754187,0.0001521054,0.00048114083,0.00085442665,0.00070493616,0.00031287313,0.00029483144,0.0032575997],"category_scores_gemma":[0.000282256,0.00008332495,0.00009585347,0.0004261063,0.00052576524,0.0002530765,0.0004784008,0.0002429517,0.0005827653],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005753826,0.00012499148,0.84321564,0.0000776625,0.000053181135,0.0062204115,0.0019508232,0.00019938448,0.10843336,0.0016126405,0.0009786803,0.03655788],"study_design_scores_gemma":[0.000008342237,0.000091198795,0.9751247,0.000015448852,0.000017340746,0.009832118,0.0007532577,0.00023649009,0.004058161,0.00022809845,0.009627513,0.000007177186],"about_ca_topic_score_codex":0.0035319019,"about_ca_topic_score_gemma":0.0054445164,"teacher_disagreement_score":0.0035319019,"about_ca_system_score_codex":0.00036507836,"about_ca_system_score_gemma":0.00015162984,"threshold_uncertainty_score":0.010897756},"labels":[],"label_agreement":null},{"id":"W4386212056","doi":"10.3847/1538-4357/aceb64","title":"Energy Budget in the Solar Corona","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Goddard Space Flight Center; Uniwersytet Wrocławski; Bundesministerium für Wirtschaft und Energie; Agenzia Spaziale Italiana; Nuclear Safety and Security Commission; Grantová Agentura České Republiky; National Aeronautics and Space Administration; Office of Experimental Program to Stimulate Competitive Research; Istituto Nazionale di Astrofisica; National Science Foundation","keywords":"Physics; Corona (planetary geology); Solar wind; Energy flux; Solar cycle; Coronal mass ejection; Nanoflares; Solar minimum; Magnetic energy; Astrophysics; Coronal loop; Coronal hole; Atmospheric sciences; Kinetic energy; Plasma; Computational physics; Astronomy; Magnetic field; Classical mechanics; Astrobiology; Nuclear physics","score_opus":0.007724777018503881,"score_gpt":0.22666653364739836,"score_spread":0.21894175662889448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386212056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99513334,0.00086539635,0.0006315707,0.00005187181,0.0000042600095,0.0000026718167,0.0003855521,0.000020576274,0.0029047239],"genre_scores_gemma":[0.998667,0.00020492484,0.00014561867,0.000010482254,0.0000035781782,0.000002155436,0.00040693898,0.000011856787,0.0005474886],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993,0.000006465197,0.0000039118454,0.000022539665,0.000015943662,0.000021056396],"domain_scores_gemma":[0.9998816,0.000033353943,0.000022412283,0.000010197828,0.000036914313,0.000015444897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010193284,0.00016251761,0.0002799517,0.0007892712,0.00019498242,0.00053705694,0.00020401845,0.00021847899,0.002303758],"category_scores_gemma":[0.00039983788,0.00011533047,0.00011823164,0.00062752527,0.00013098957,0.00066490215,0.00033022667,0.00011052988,0.00026603744],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009561791,0.00009373187,0.6612206,0.00033633967,0.0004693021,0.00087225984,0.00032606156,0.0325227,0.20441276,0.007681522,0.0013361812,0.08977221],"study_design_scores_gemma":[0.000029605371,0.00013619495,0.9409502,0.000049087448,0.00009073431,0.00042482885,0.00026407998,0.02564702,0.021980545,0.003988613,0.0064103976,0.000028712493],"about_ca_topic_score_codex":0.002114729,"about_ca_topic_score_gemma":0.0017660597,"teacher_disagreement_score":0.002303758,"about_ca_system_score_codex":0.00023173547,"about_ca_system_score_gemma":0.00013476616,"threshold_uncertainty_score":0.007706821},"labels":[],"label_agreement":null},{"id":"W4386250645","doi":"10.3847/1538-4357/ace720","title":"As Simple as Possible but No Simpler: Optimizing the Performance of Neural Net Emulators for Galaxy SED Fitting","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Emulation; Galaxy; Physics; Artificial neural network; Outlier; Metallicity; Astrophysics; Algorithm; Computer science; Artificial intelligence","score_opus":0.01115912920814967,"score_gpt":0.24117655405755672,"score_spread":0.23001742484940704,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386250645","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6977736,0.00037378806,0.29058158,0.000609281,0.00006033079,0.0001049651,0.00017146663,0.0045806617,0.005744284],"genre_scores_gemma":[0.90448326,0.000049204416,0.094158754,0.00013473764,0.000008440278,0.000057620444,0.00012205626,0.00020717907,0.0007788566],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99976057,0.00011069916,0.000012417935,0.000043585133,0.00003648379,0.000036229438],"domain_scores_gemma":[0.9983942,0.0011518507,0.00009893461,0.00011608156,0.0001592237,0.0000797416],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015739279,0.00080933195,0.00031839695,0.00040821257,0.000293548,0.0006070863,0.0009487542,0.0006634959,0.0016129123],"category_scores_gemma":[0.006110421,0.00032225548,0.00031625386,0.00032527887,0.00042892725,0.0007741278,0.00049360096,0.00082939636,0.0003823475],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009462203,0.000052853728,0.0025250153,0.000022972026,0.000035052853,0.000024631549,0.000019672249,0.97341114,0.0020278273,0.00088349223,0.0003944242,0.020508364],"study_design_scores_gemma":[0.000005300186,0.0000138615,0.00018504927,0.0000033650983,0.000003568272,0.0000029594487,0.0000065246886,0.998071,0.0013457037,0.00025942383,0.00010119972,0.0000020027496],"about_ca_topic_score_codex":0.0067068394,"about_ca_topic_score_gemma":0.0070126923,"teacher_disagreement_score":0.0067068394,"about_ca_system_score_codex":0.0009467396,"about_ca_system_score_gemma":0.00081120204,"threshold_uncertainty_score":0.013335586},"labels":[],"label_agreement":null},{"id":"W4386250715","doi":"10.3847/1538-4357/ace961","title":"Technical Constraints on Interstellar Interferometry and Spatially Resolving the Pulsar Magnetosphere","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Pulsar; Millisecond pulsar; Magnetosphere; Astrophysics; Astronomy; Interstellar medium; Scintillation; Interferometry; Radio telescope; Binary pulsar; Optics; Magnetic field","score_opus":0.011506046567480084,"score_gpt":0.232820117933039,"score_spread":0.22131407136555892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386250715","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.868004,0.004121872,0.10802226,0.0015631707,0.0001228705,0.00009110424,0.001231695,0.0005169786,0.016326174],"genre_scores_gemma":[0.94076663,0.0012341806,0.055447627,0.00026613276,0.0000999214,0.000125906,0.0008261468,0.00010483794,0.0011286484],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99830735,0.0006143882,0.00019005759,0.00021652972,0.00053844746,0.00013330039],"domain_scores_gemma":[0.98721355,0.007147372,0.002049503,0.0020961445,0.0011542226,0.0003392346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0035919414,0.000344599,0.00039077387,0.00086870167,0.00041080898,0.0011279227,0.00083249505,0.00046241397,0.002497507],"category_scores_gemma":[0.012312186,0.00026943264,0.00023689485,0.0011095918,0.0005823816,0.0011956259,0.0010854846,0.00042958668,0.0007399747],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009842841,0.00010440205,0.17132528,0.00058243837,0.00012783862,0.0008374396,0.0004590051,0.0074611357,0.72014105,0.022313192,0.0011783455,0.07448556],"study_design_scores_gemma":[0.00011328846,0.0012449651,0.5500706,0.00030383904,0.0003724724,0.004192797,0.001270831,0.02684283,0.3636143,0.01414838,0.037700932,0.00012483154],"about_ca_topic_score_codex":0.0015927107,"about_ca_topic_score_gemma":0.0031677717,"teacher_disagreement_score":0.0035919414,"about_ca_system_score_codex":0.00047946034,"about_ca_system_score_gemma":0.00084582425,"threshold_uncertainty_score":0.018996239},"labels":[],"label_agreement":null},{"id":"W4386255904","doi":"10.3847/1538-4357/ace9b8","title":"A Tale of Two Disks: Mapping the Milky Way with the Final Data Release of APOGEE","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Office of International Science and Engineering; Office of Science; Agencia Nacional de Investigación y Desarrollo; Banco Santander; Alfred P. Sloan Foundation; U.S. Department of Energy; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; National Science Foundation","keywords":"Physics; Milky Way; Metallicity; Astrophysics; Thick disk; Thin disk; Disc; Astronomy; Galaxy; Stellar population; Galactic plane; Galaxy formation and evolution; RADIUS; Stars; Population; Star formation; Demography; Halo","score_opus":0.04199217264137052,"score_gpt":0.25747621400951576,"score_spread":0.21548404136814525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386255904","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99790204,0.000099152225,0.00017628423,0.000048401667,0.0000032790695,0.0000038532817,0.0012453833,0.000019588799,0.00050200825],"genre_scores_gemma":[0.9943863,0.00006218041,0.0009715249,0.000028672313,0.0000081739545,0.000010558441,0.004006398,0.000025426161,0.0005007434],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995697,0.000058397025,0.000030083473,0.00016060018,0.00010309079,0.00007814989],"domain_scores_gemma":[0.99838316,0.00017141717,0.000529969,0.0003378522,0.00030656988,0.00027098026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005049389,0.00023328615,0.0003387806,0.0021295594,0.00032514648,0.001156024,0.00030858038,0.00028352227,0.0006133596],"category_scores_gemma":[0.0016422785,0.0001882275,0.00024341635,0.001795403,0.00032317944,0.000648431,0.0015754319,0.00023719344,0.00031796316],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015260963,0.000030099889,0.97953564,0.00003149722,0.0001215665,0.00018223363,0.0010469353,0.00027995903,0.007194456,0.0001528329,0.0011597894,0.010112487],"study_design_scores_gemma":[0.0000042573497,0.000021288453,0.99628145,0.000005990945,0.000015841508,0.00008421264,0.00043592908,0.00025765208,0.00046603495,0.000049673097,0.0023719824,0.0000057130346],"about_ca_topic_score_codex":0.012687144,"about_ca_topic_score_gemma":0.02367883,"teacher_disagreement_score":0.012687144,"about_ca_system_score_codex":0.00036407117,"about_ca_system_score_gemma":0.00026504096,"threshold_uncertainty_score":0.025226593},"labels":[],"label_agreement":null},{"id":"W4386269533","doi":"10.3847/1538-4357/ad1eed","title":"A Joint Fermi-GBM and Swift-BAT Analysis of Gravitational-wave Candidates from the Third Gravitational-wave Observing Run","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; University of British Columbia; Perimeter Institute; University of Toronto","funders":"European Social Fund; National Research, Development and Innovation Office; Institute for Cosmic Ray Research, University of Tokyo; Japan Society for the Promotion of Science; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Marshall Space Flight Center; National Science and Technology Council; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, India; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Hungarian Scientific Research Fund; Generalitat Valenciana; Generalitat de Catalunya; Great Southern Development Commission, Government of Western Australia; Agencia Estatal de Investigación; Govern de les Illes Balears; Korea Institute of Science and Technology Information; Ministry of Education, Culture, Sports, Science and Technology; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Council of Scientific and Industrial Research, India; Universities Space Research Association; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Vetenskapsrådet; U.S. Department of Energy; Ministerio de Ciencia e Innovación; Leverhulme Trust; European Commission; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Russian Science Foundation; Scottish Funding Council; HORIZON EUROPE Marie Sklodowska-Curie Actions; Institut des Origines de Lyon; Centres de Recerca de Catalunya; Fonds Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; Fermi Gamma-ray Space Telescope; Gamma-ray burst; Astrophysics; LIGO; Gravitational wave; Luminosity; Neutron star; Astronomy; Swift; Galaxy","score_opus":0.027461768508746414,"score_gpt":0.30366075507750984,"score_spread":0.2761989865687634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386269533","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972572,0.000030114163,0.0007977945,0.000018478266,0.0000021279054,0.000009106138,0.0011343225,0.00006073217,0.00069027167],"genre_scores_gemma":[0.99487174,0.000018766388,0.0011975735,0.0000129051095,0.0000041729877,0.000009331254,0.0034552554,0.000024809602,0.00040547867],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976784,0.000030270818,0.000012731631,0.00004413696,0.00007530782,0.00006964436],"domain_scores_gemma":[0.99918205,0.00014220197,0.00023813802,0.000097598364,0.000145546,0.00019448645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042736006,0.0003180978,0.0004032514,0.001715904,0.00035136257,0.0005624726,0.0002705924,0.00023915933,0.0010262458],"category_scores_gemma":[0.0006181296,0.00012927914,0.000784389,0.0010112822,0.00017792912,0.00018422338,0.00062544685,0.00022729028,0.0003187985],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006008499,0.00008375347,0.95625407,0.000025964526,0.00024085793,0.0006827612,0.00026107658,0.0052887253,0.01985542,0.0007429376,0.0012011555,0.014762375],"study_design_scores_gemma":[0.000019998162,0.00010152362,0.9824256,0.0000070299047,0.00009717459,0.00032288145,0.00013790077,0.011507163,0.0040124124,0.00024291367,0.0011093776,0.000016071153],"about_ca_topic_score_codex":0.012408793,"about_ca_topic_score_gemma":0.022666246,"teacher_disagreement_score":0.012408793,"about_ca_system_score_codex":0.00034096657,"about_ca_system_score_gemma":0.0004216993,"threshold_uncertainty_score":0.024673104},"labels":[],"label_agreement":null},{"id":"W4386307905","doi":"10.3847/1538-4357/ace629","title":"Sudden Extreme Obscuration of a Sun-like Main-sequence Star: Evolution of the Circumstellar Dust around ASASSN-21qj","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"HORIZON EUROPE Marie Sklodowska-Curie Actions; Agencia Estatal de Investigación; Ministerio de Ciencia e Innovación; Ministry of Science and Technology, Taiwan; Space Telescope Science Institute; Consejo Nacional de Ciencia y Tecnología; National Aeronautics and Space Administration; European Space Agency; Queen's University Belfast; Science and Technology Facilities Council; Queen's University; European Commission; Nuclear Safety and Security Commission","keywords":"Physics; Astrophysics; Stars","score_opus":0.031174584586070867,"score_gpt":0.23877031521450967,"score_spread":0.2075957306284388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386307905","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992918,0.000027931274,0.000047690697,0.000012272398,0.0000018492996,0.0000019508182,0.000089760455,0.0000063012476,0.0005203668],"genre_scores_gemma":[0.99918216,0.000016955204,0.000118731856,0.0000143311345,0.0000033156161,0.0000021018895,0.0003562666,0.000005144473,0.00030092595],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999429,0.000004231196,0.0000024105411,0.000017243116,0.000019145418,0.000014054884],"domain_scores_gemma":[0.9998474,0.0000095910345,0.000028387361,0.000009199273,0.000023883205,0.000081595346],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011912964,0.00014694125,0.00021708527,0.00036073857,0.0005216331,0.00046928573,0.0001589798,0.00023403294,0.0007594448],"category_scores_gemma":[0.00021198762,0.00013366221,0.00012955112,0.00022610923,0.00024446205,0.00016566145,0.0004595566,0.00024702365,0.00023397003],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018817147,0.00006233742,0.8701729,0.000033823104,0.00005814666,0.0018215425,0.0010815273,0.0005309098,0.11921456,0.00020660521,0.00077165046,0.0058578495],"study_design_scores_gemma":[0.0000026992923,0.000026678714,0.99815,0.0000014503546,0.0000037904988,0.00014085043,0.00015853423,0.0002904988,0.0007479291,0.000020488545,0.00045470375,0.0000024943286],"about_ca_topic_score_codex":0.0067369156,"about_ca_topic_score_gemma":0.014878899,"teacher_disagreement_score":0.0067369156,"about_ca_system_score_codex":0.00037408096,"about_ca_system_score_gemma":0.00013593856,"threshold_uncertainty_score":0.013395369},"labels":[],"label_agreement":null},{"id":"W4386357093","doi":"10.3847/1538-4357/ace52f","title":"Limits on Fast Radio Burst–like Counterparts to Gamma-Ray Bursts Using CHIME/FRB","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"McGill Space Institute; Smithsonian Astrophysical Observatory; University of Toronto; McGill University; Canadian Institute for Advanced Research","keywords":"Physics; Astrophysics; Fermi Gamma-ray Space Telescope; Fast radio burst; Gamma-ray burst; Flux (metallurgy); Astronomy; Neutron star","score_opus":0.024889943232501138,"score_gpt":0.33411566063511716,"score_spread":0.309225717402616,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386357093","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96814346,0.0009005084,0.011195258,0.00019725763,0.000016100366,0.00006391047,0.009428252,0.00078063796,0.0092745675],"genre_scores_gemma":[0.9789665,0.00013752877,0.007705107,0.00007025763,0.000009832389,0.000027475315,0.012486701,0.00008752847,0.00050914503],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99888283,0.00012282166,0.000034440487,0.0004035414,0.0003466345,0.0002097076],"domain_scores_gemma":[0.9960962,0.0011412055,0.0008848927,0.0007933875,0.00052095944,0.0005634626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023578217,0.00060398586,0.00053663173,0.0024538857,0.00068181084,0.001312327,0.000942938,0.00067148777,0.0019290999],"category_scores_gemma":[0.0047889813,0.00038238885,0.0004903359,0.0017429995,0.00048818745,0.00063506747,0.0013722294,0.00037885038,0.0007152219],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055010564,0.00008346603,0.94298786,0.00012853637,0.00027908615,0.000310456,0.00029301277,0.009447795,0.02042087,0.0011226549,0.0019013439,0.022474667],"study_design_scores_gemma":[0.000023570234,0.000053613974,0.9644629,0.00005040252,0.00007297162,0.00030723723,0.00019770757,0.02379227,0.0037585543,0.000533381,0.006700108,0.00004722522],"about_ca_topic_score_codex":0.11178944,"about_ca_topic_score_gemma":0.12530774,"teacher_disagreement_score":0.11178944,"about_ca_system_score_codex":0.0010090306,"about_ca_system_score_gemma":0.0008374231,"threshold_uncertainty_score":0.22227752},"labels":[],"label_agreement":null},{"id":"W4386457390","doi":"10.3847/1538-4357/acddda","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: The Black Hole Mass–Stellar Mass Relations at 0.2 ≲ z ≲ 0.8","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Galaxy; Quasar; Astrophysics; Redshift; Black hole (networking); Stellar mass; Star formation","score_opus":0.016566346950416293,"score_gpt":0.22464786313560484,"score_spread":0.20808151618518855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386457390","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9876046,0.00009723941,0.00035344478,0.00009444886,0.000004816517,0.000010840357,0.009685131,0.00007069624,0.0020786133],"genre_scores_gemma":[0.97723335,0.000072780575,0.0007605969,0.000038497194,0.000012682841,0.000020634205,0.020815408,0.000037455724,0.0010086338],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99969864,0.000072062314,0.000016328127,0.00006267083,0.0000870995,0.000063162486],"domain_scores_gemma":[0.99818724,0.00013960383,0.0007098855,0.00027367272,0.00035053582,0.0003389487],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010818101,0.00025782984,0.00018099825,0.0017797125,0.00021456303,0.0005285562,0.00026066092,0.00013982353,0.0015622907],"category_scores_gemma":[0.0017250732,0.00010686697,0.00014647457,0.0014563065,0.0001608279,0.00030802807,0.00065832085,0.00017093633,0.0008366179],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008347639,0.000028330076,0.986389,0.000012016045,0.000042212014,0.00004766995,0.00022010412,0.0002888219,0.00070463377,0.00013686897,0.0044756676,0.007571172],"study_design_scores_gemma":[0.0000025605677,0.000006287446,0.9984999,0.0000017837667,0.0000037616232,0.0000199607,0.00005317972,0.00021780991,0.0001427705,0.000022364264,0.0010279045,0.0000016478356],"about_ca_topic_score_codex":0.017832078,"about_ca_topic_score_gemma":0.02313017,"teacher_disagreement_score":0.017832078,"about_ca_system_score_codex":0.00026385242,"about_ca_system_score_gemma":0.00021642847,"threshold_uncertainty_score":0.03545654},"labels":[],"label_agreement":null},{"id":"W4386482639","doi":"10.3847/1538-4357/acea83","title":"Three-dimensional General-relativistic Simulations of Neutrino-driven Winds from Magnetized Proto–Neutron Stars","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Neutron star; Ejecta; Outflow; Supernova; Neutrino; Astrophysics; Nucleosynthesis; Field line; Magnetic field; Dipole; Polar; Magnetosphere; Plasma; Astronomy; Nuclear physics","score_opus":0.018693654045210985,"score_gpt":0.3097395817570596,"score_spread":0.2910459277118486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386482639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9884715,0.00012800201,0.0019773857,0.00036983902,0.00007294621,0.000045593846,0.0005805692,0.00016631902,0.008187833],"genre_scores_gemma":[0.99638677,0.00007462099,0.0017092568,0.00010127291,0.000022127178,0.000033505043,0.00049251504,0.000046203455,0.0011337469],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998522,0.00004091107,0.0000071597087,0.00001972394,0.000027180828,0.000052797895],"domain_scores_gemma":[0.99912983,0.00038093684,0.000114004004,0.000043881388,0.00010054104,0.0002308065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004128113,0.0006060208,0.0007073295,0.0004645397,0.0008224549,0.00093579583,0.0014051154,0.0015334755,0.0031814747],"category_scores_gemma":[0.0016237414,0.00051473477,0.0009903503,0.0005622352,0.001175256,0.00036575456,0.00083654054,0.0013752105,0.00023483807],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028066302,0.00021283794,0.0056634727,0.00003756813,0.000098208206,0.00022359108,0.000084970314,0.98918086,0.0011895559,0.0015591729,0.0005114896,0.00095771643],"study_design_scores_gemma":[0.00011941068,0.00009066482,0.002852924,0.0000075762787,0.000019337003,0.000017887882,0.0000641062,0.99579453,0.00024912256,0.0004514939,0.00032210306,0.000010810332],"about_ca_topic_score_codex":0.040134322,"about_ca_topic_score_gemma":0.023283914,"teacher_disagreement_score":0.040134322,"about_ca_system_score_codex":0.0012044676,"about_ca_system_score_gemma":0.0010228846,"threshold_uncertainty_score":0.07980138},"labels":[],"label_agreement":null},{"id":"W4386515691","doi":"10.3847/1538-4357/ace90a","title":"The DESI One-Percent Survey: Constructing Galaxy–Halo Connections for ELGs and LRGs Using Auto and Cross Correlations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Division of Astronomical Sciences; Jet Propulsion Laboratory; Office of Science; Science and Technology Facilities Council; Higher Education Discipline Innovation Project; Ministerio de Ciencia e Innovación; Chinese Academy of Sciences; National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation; Heising-Simons Foundation; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; National Natural Science Foundation of China; University of California; Consejo Nacional de Ciencia y Tecnología; Shanghai Jiao Tong University; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Halo; Redshift; Dark matter; Dark matter halo; Stellar mass; Astronomy; Star formation","score_opus":0.030746601505057845,"score_gpt":0.27399728619370706,"score_spread":0.24325068468864922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386515691","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99193645,0.0000410586,0.0056307768,0.000027031863,0.0000016953552,0.000008100507,0.001360311,0.00016464811,0.0008299458],"genre_scores_gemma":[0.9955367,0.000015401614,0.0025564579,0.0000093723465,0.0000025739369,0.000008643247,0.0017275348,0.000024934143,0.00011832259],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996793,0.0001109271,0.000010782313,0.00009795109,0.00005377057,0.00004730457],"domain_scores_gemma":[0.9979761,0.00051305845,0.0005219093,0.00047229853,0.0002579287,0.00025874938],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010912727,0.00033008002,0.0002603599,0.0019396206,0.00025263338,0.0005531927,0.0005829939,0.00026919311,0.0008794235],"category_scores_gemma":[0.0029269324,0.0002558256,0.00052747113,0.0015771112,0.00026598267,0.0004129969,0.00073533005,0.00028465714,0.0002433834],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008987797,0.000025467998,0.9521477,0.000017209155,0.00012708521,0.00004886683,0.000083770035,0.035428837,0.0015179832,0.0017544727,0.0009040627,0.007854682],"study_design_scores_gemma":[0.000013411289,0.000023593911,0.8034514,0.0000075659846,0.000022173117,0.0000595845,0.000075423726,0.19297752,0.0014144492,0.0010447572,0.00089352595,0.000016710257],"about_ca_topic_score_codex":0.015658591,"about_ca_topic_score_gemma":0.019099878,"teacher_disagreement_score":0.015658591,"about_ca_system_score_codex":0.0006676462,"about_ca_system_score_gemma":0.00027254072,"threshold_uncertainty_score":0.031134903},"labels":[],"label_agreement":null},{"id":"W4386563139","doi":"10.3847/1538-4357/ace9d9","title":"Investigating the Lower Mass Gap with Low-mass X-Ray Binary Population Synthesis","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; European Commission; China Scholarship Council; Flatiron Health; Canadian Institute for Advanced Research; Simons Foundation; Northwestern University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Physics; Binary number; Astrophysics; Astronomy; Population; X-ray binary; Low Mass; Neutron star; Stars; Medicine","score_opus":0.02071440784508946,"score_gpt":0.26956260277496796,"score_spread":0.2488481949298785,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386563139","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99798775,0.000025972386,0.0015837881,0.000013377002,8.522159e-7,0.0000036476017,0.000058120073,0.000013586906,0.00031290267],"genre_scores_gemma":[0.9991504,0.000010904451,0.0006568363,0.000007747856,7.702132e-7,0.0000046211026,0.0001024542,0.000005559324,0.000060704657],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985087,0.00004547557,0.000008659834,0.000051973326,0.000024011615,0.000019060511],"domain_scores_gemma":[0.99884075,0.0005848149,0.00025869784,0.00016008623,0.000099819874,0.000055896664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065046153,0.00015964881,0.00022094022,0.00024762,0.00014188232,0.0005294679,0.00030770726,0.00021410691,0.0007392714],"category_scores_gemma":[0.0032414494,0.00011667187,0.00015420259,0.00022650951,0.00021201531,0.0004383829,0.00037911828,0.00015866132,0.000113818955],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042492175,0.0001639221,0.7650063,0.00013218928,0.0001912934,0.00026017672,0.00048467392,0.1299491,0.065705195,0.01177175,0.00048055992,0.02542985],"study_design_scores_gemma":[0.00003659949,0.0002341667,0.23644435,0.000016946891,0.00007365213,0.00018187195,0.00021223661,0.7123738,0.044322643,0.0046371575,0.001447464,0.000019132598],"about_ca_topic_score_codex":0.0016181722,"about_ca_topic_score_gemma":0.0011093398,"teacher_disagreement_score":0.0016181722,"about_ca_system_score_codex":0.00049011444,"about_ca_system_score_gemma":0.00017903496,"threshold_uncertainty_score":0.0035560727},"labels":[],"label_agreement":null},{"id":"W4386615376","doi":"10.3847/1538-4357/aced92","title":"A Reemerging Bright Soft X-Ray State of the Changing-look Active Galactic Nucleus 1ES 1927+654: A Multiwavelength View","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Goddard Space Flight Center; Hungarian Scientific Research Fund; National Natural Science Foundation of China; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; European Commission; National Aeronautics and Space Administration; National Research, Development and Innovation Office; National Science Foundation","keywords":"Physics; Astrophysics; Active galactic nucleus; Supermassive black hole; Accretion (finance); Flare; Flux (metallurgy); Astronomy; Accretion disc; Black hole (networking); Galaxy","score_opus":0.013210768916224976,"score_gpt":0.23766034547170967,"score_spread":0.2244495765554847,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386615376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958825,0.00020338524,0.00020736916,0.00006331565,0.000009031032,0.0000030435162,0.0002558563,0.00002901352,0.0033464048],"genre_scores_gemma":[0.9983633,0.000058325877,0.00019396235,0.000031753418,0.000018410165,0.0000015929182,0.00031984414,0.000007896764,0.0010047872],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999969,0.0000019010869,0.0000014931951,0.000010944612,0.000006962686,0.000009723837],"domain_scores_gemma":[0.99991,0.000004959171,0.000031269537,0.0000075928187,0.00001381061,0.00003236788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006680126,0.00011658402,0.00010858645,0.0008334272,0.0002883927,0.0005123028,0.00018604225,0.00020433657,0.0019276848],"category_scores_gemma":[0.00008557967,0.00010158226,0.00016012922,0.00028781535,0.00019163275,0.00022446901,0.00033741715,0.0002404399,0.0003074768],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004834384,0.00011200858,0.75081354,0.00006734652,0.00010327634,0.0037285793,0.00081443036,0.00043239284,0.21930318,0.0007379944,0.0017795641,0.02162422],"study_design_scores_gemma":[0.0000031481923,0.0000324701,0.9955695,0.0000041822436,0.000012241538,0.0008197953,0.00019547029,0.00026246396,0.001672884,0.00007836754,0.0013450906,0.0000043462746],"about_ca_topic_score_codex":0.0044681807,"about_ca_topic_score_gemma":0.0074147154,"teacher_disagreement_score":0.0044681807,"about_ca_system_score_codex":0.00030318205,"about_ca_system_score_gemma":0.00007727333,"threshold_uncertainty_score":0.008884311},"labels":[],"label_agreement":null},{"id":"W4386636207","doi":"10.3847/1538-4357/acebc0","title":"GHOST Commissioning Science Results: Identifying a New Chemically Peculiar Star in Reticulum II","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Spectrograph; Stars; Astrophysics; Astronomy; Telescope; Galaxy; Supernova; Dwarf galaxy; Spectral resolution; Spectral line","score_opus":0.01921560165535568,"score_gpt":0.2661726153857543,"score_spread":0.24695701373039863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386636207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995201,0.0001452509,0.0009402436,0.00011734654,0.000026384838,0.000020459149,0.00064850325,0.00019236967,0.0027084607],"genre_scores_gemma":[0.9955914,0.000030452264,0.00235077,0.000097955235,0.000014522428,0.000005122575,0.0010962664,0.000043965872,0.00076960446],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995845,0.000029483363,0.00002573469,0.00013274368,0.00016085547,0.00006667875],"domain_scores_gemma":[0.99871564,0.000104102335,0.00026999618,0.00028387495,0.00018897565,0.00043746538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00094233715,0.00024491324,0.0003386769,0.0011900947,0.0008335972,0.0011399948,0.00032361445,0.00040056277,0.00076693564],"category_scores_gemma":[0.00093997567,0.00019546044,0.00026692057,0.0007474216,0.00052514364,0.0005337908,0.001551127,0.0004767844,0.0002827613],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066947564,0.00016325623,0.85004216,0.000098060904,0.000101027814,0.0016314643,0.0016755753,0.0006874351,0.110258594,0.0014154814,0.003097994,0.030159544],"study_design_scores_gemma":[0.000030443807,0.000378071,0.95497215,0.000012187091,0.00005338649,0.0012497035,0.00048090913,0.0014802319,0.02485473,0.00047237697,0.01598401,0.0000318554],"about_ca_topic_score_codex":0.0029443717,"about_ca_topic_score_gemma":0.005779493,"teacher_disagreement_score":0.0029443717,"about_ca_system_score_codex":0.00082679,"about_ca_system_score_gemma":0.00037725127,"threshold_uncertainty_score":0.0059987903},"labels":[],"label_agreement":null},{"id":"W4386636296","doi":"10.3847/1538-4357/acdc96","title":"The EB Correlation in Resolved Polarized Images: Connections to the Astrophysics of Black Holes","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Harvard University","keywords":"Physics; Astrophysics; Correlation function (quantum field theory); Magnetic field; Faraday effect; Polarization (electrochemistry); Computational physics; Quantum mechanics","score_opus":0.016067455944060578,"score_gpt":0.24832533529664466,"score_spread":0.23225787935258407,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386636296","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97246593,0.00014010347,0.024920711,0.0001545524,0.000014561891,0.000014798078,0.00012731309,0.00010410939,0.0020578895],"genre_scores_gemma":[0.9985355,0.00002494351,0.0013002296,0.0000060080447,0.0000053180274,0.0000021236121,0.00003501333,0.000021708884,0.00006919192],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999013,0.00003267124,0.000003893756,0.000016893715,0.000020768986,0.00002441662],"domain_scores_gemma":[0.99962425,0.00012912923,0.000096771546,0.00005733103,0.000042731805,0.00004969069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042166052,0.00027600364,0.00021426434,0.00064282765,0.00021885593,0.0007080262,0.00033365327,0.00027448242,0.000683821],"category_scores_gemma":[0.0018362321,0.00017402752,0.00031407006,0.0003134903,0.00066122715,0.0006253029,0.00041269406,0.00030929374,0.00005246092],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002775742,0.00010264509,0.047515903,0.00009103439,0.000109808534,0.00042714286,0.0002561219,0.87597543,0.03461578,0.02980812,0.00069251616,0.010127906],"study_design_scores_gemma":[0.000011662228,0.000027149621,0.012296477,0.000005830249,0.0000071154936,0.000047596386,0.00004114876,0.98094016,0.002535815,0.00383128,0.0002453991,0.000010358336],"about_ca_topic_score_codex":0.0020226366,"about_ca_topic_score_gemma":0.0006755975,"teacher_disagreement_score":0.0020226366,"about_ca_system_score_codex":0.00034183558,"about_ca_system_score_gemma":0.00022937152,"threshold_uncertainty_score":0.004021704},"labels":[],"label_agreement":null},{"id":"W4386691212","doi":"10.3847/1538-4357/ace7b7","title":"The HERBAL Model: A Hierarchical Errors-in-variables Bayesian Lognormal Hurdle Model for Galactic Globular Cluster Populations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; University of Toronto; Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Globular cluster; Astrophysics; Galaxy; Dwarf galaxy; Luminosity; Stellar mass; Stellar population; Population; Log-normal distribution; Statistics; Star formation; Mathematics; Medicine","score_opus":0.018326063932544674,"score_gpt":0.2545951645237146,"score_spread":0.23626910059116993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386691212","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.21135958,0.0011448789,0.7632797,0.0035184652,0.00019642527,0.00033969228,0.003610308,0.0011961891,0.015354722],"genre_scores_gemma":[0.9082983,0.00072322943,0.06337662,0.00089865975,0.0003120044,0.0005279873,0.002280843,0.0004884451,0.02309383],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9971776,0.0013074073,0.00010602332,0.0006389779,0.00031458974,0.0004554741],"domain_scores_gemma":[0.98793507,0.007406792,0.001382177,0.00092185166,0.0017138902,0.00064021506],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007100102,0.0011904769,0.0023472044,0.0021412992,0.0014780803,0.0037004943,0.0067545483,0.0025340216,0.0077610575],"category_scores_gemma":[0.024855973,0.0012955428,0.00211001,0.0018733302,0.0023380828,0.00423088,0.0024864895,0.003097155,0.0020199183],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016335487,0.00008827803,0.018683337,0.00006573894,0.00016669085,0.00028337038,0.00046158957,0.786715,0.00035191665,0.17337216,0.006193254,0.01345535],"study_design_scores_gemma":[0.00003636823,0.00001800564,0.0017834351,0.000019081677,0.000033888577,0.000054151984,0.000053985277,0.9511687,0.000055328677,0.045717284,0.0010300898,0.000029625362],"about_ca_topic_score_codex":0.07749885,"about_ca_topic_score_gemma":0.047680713,"teacher_disagreement_score":0.07749885,"about_ca_system_score_codex":0.0035458296,"about_ca_system_score_gemma":0.0018698571,"threshold_uncertainty_score":0.15409553},"labels":[],"label_agreement":null},{"id":"W4386691418","doi":"10.3847/1538-4357/acefb6","title":"Chance Coincidences between Black Hole Low-mass X-Ray Binaries and Supernova Remnants","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Low Mass; Supernova; Black hole (networking); Binary number; Swift; Astronomy; Stars","score_opus":0.022193761328618392,"score_gpt":0.25345929727061234,"score_spread":0.23126553594199395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386691418","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9905973,0.00096991064,0.0028280104,0.00039766924,0.000113537535,0.000018696133,0.00012187516,0.0000494545,0.0049036476],"genre_scores_gemma":[0.9990671,0.00011416472,0.00040479656,0.000055802953,0.00007279604,0.000003997045,0.00007079123,0.0000031278016,0.00020742687],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9977156,0.00064804277,0.00028754777,0.0007001569,0.00044565607,0.00020298708],"domain_scores_gemma":[0.9769106,0.012505854,0.0059530945,0.0023941179,0.00071737316,0.001519013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0033396913,0.00020870731,0.00037238607,0.0015722361,0.00073521544,0.0018886917,0.0005470875,0.0011691615,0.0050726244],"category_scores_gemma":[0.019384556,0.00034611023,0.00029951523,0.001011538,0.0014083016,0.0013190303,0.0016127456,0.0007320369,0.0006760506],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053024077,0.000036792593,0.9831104,0.000040767423,0.000114536306,0.0044277823,0.00027633237,0.00022689093,0.0016201028,0.0032046053,0.00041524277,0.0059961965],"study_design_scores_gemma":[0.000088046625,0.00061561697,0.90566814,0.000077810924,0.0002296484,0.05914933,0.001750578,0.0035477157,0.005769538,0.01894901,0.004066475,0.000088130466],"about_ca_topic_score_codex":0.00046475139,"about_ca_topic_score_gemma":0.00051837583,"teacher_disagreement_score":0.0050726244,"about_ca_system_score_codex":0.00020616263,"about_ca_system_score_gemma":0.0001395385,"threshold_uncertainty_score":0.017662168},"labels":[],"label_agreement":null},{"id":"W4386691736","doi":"10.3847/1538-4357/acebc5","title":"A Wideband Polarization Observation of Hydra A with the Jansky Very Large Array","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Faraday effect; Polarization (electrochemistry); Depolarization; Magnetic field; Faraday cage; Astrophysics; Computational physics","score_opus":0.009472639549814985,"score_gpt":0.2116628766680028,"score_spread":0.20219023711818782,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386691736","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99629956,0.00011488998,0.0012563028,0.00003591048,0.000007918288,0.000009001222,0.0003068493,0.00007171854,0.0018979126],"genre_scores_gemma":[0.997954,0.000049831186,0.0013030912,0.000026770595,0.000018097262,0.0000047137637,0.0002837494,0.00001005066,0.00034959568],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992657,0.000009694441,0.000002336873,0.00002180374,0.00001876886,0.000020831501],"domain_scores_gemma":[0.9998472,0.000025535577,0.000029862487,0.000027284186,0.000021630136,0.000048502305],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018267552,0.00016110647,0.00017832826,0.00041788502,0.00037992548,0.00036240552,0.00016480817,0.00020229506,0.00057569],"category_scores_gemma":[0.00019907413,0.00018411221,0.00019951937,0.00022039485,0.00022601032,0.0002163676,0.00048194153,0.00030429053,0.00026188552],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005653709,0.00017042992,0.16675831,0.00006758255,0.00020277791,0.0014499273,0.00038410808,0.001688318,0.810312,0.0007301394,0.0010705495,0.016600557],"study_design_scores_gemma":[0.000042692223,0.00028046226,0.967512,0.000008528712,0.00008591468,0.0009500638,0.00018813567,0.0031120526,0.023236234,0.00028455822,0.0042708595,0.000028390024],"about_ca_topic_score_codex":0.0012699884,"about_ca_topic_score_gemma":0.0019519262,"teacher_disagreement_score":0.0012699884,"about_ca_system_score_codex":0.00010599468,"about_ca_system_score_gemma":0.000087209104,"threshold_uncertainty_score":0.0025252104},"labels":[],"label_agreement":null},{"id":"W4386742172","doi":"10.3847/1538-4357/ace976","title":"Orbital Support and Evolution of Flat Profiles of Bars (Shoulders)","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Science and Technology Facilities Council; Nuclear Safety and Security Commission; Flatiron Health; University of Central Lancashire; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Shoulders; Astrophysics; Orbital plane; Astronomy; Classical mechanics","score_opus":0.011964267699819536,"score_gpt":0.23579095341068676,"score_spread":0.22382668571086722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386742172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998569,0.00002707384,0.00056269334,0.000017265218,0.0000018893205,0.0000023722891,0.000040191062,0.000031534622,0.00074796943],"genre_scores_gemma":[0.9995977,0.0000070572446,0.00023214822,0.0000041846497,7.653114e-7,0.0000014671665,0.000043281438,0.00000647301,0.00010704722],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994016,0.000009251394,0.0000030898316,0.000014438097,0.00001001052,0.000023003837],"domain_scores_gemma":[0.9993678,0.00015908103,0.00016575951,0.00006997266,0.00008120293,0.00015624266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002396142,0.00017023578,0.00017055993,0.00079165975,0.0003917429,0.00061890774,0.00031040475,0.00037011885,0.001542528],"category_scores_gemma":[0.0015592849,0.00022260008,0.00033409984,0.00024327646,0.0003945662,0.00031638955,0.0004775934,0.00026873534,0.00018820021],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00078780873,0.00022741013,0.4342941,0.000096054864,0.00021891946,0.0007751664,0.00078809995,0.47338322,0.062387243,0.00604029,0.0012028193,0.019798947],"study_design_scores_gemma":[0.00006751171,0.0002732702,0.17643349,0.0000424053,0.000056456585,0.00020992635,0.0003711047,0.8141605,0.0058292695,0.0017898618,0.0007243064,0.000041819712],"about_ca_topic_score_codex":0.0060616173,"about_ca_topic_score_gemma":0.004626074,"teacher_disagreement_score":0.0060616173,"about_ca_system_score_codex":0.00050027604,"about_ca_system_score_gemma":0.00021673077,"threshold_uncertainty_score":0.012052655},"labels":[],"label_agreement":null},{"id":"W4386742301","doi":"10.3847/1538-4357/acec3a","title":"Using Giant Pulses to Measure the Impulse Response of the Interstellar Medium","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"High-pressure geophysics and materials","field":"Earth and Planetary Sciences","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Council for the Arts","keywords":"Physics; Impulse response; Impulse (physics); Deconvolution; Pulsar; Astrophysics; Computational physics; Optics; Mathematical analysis","score_opus":0.027987181357999255,"score_gpt":0.24362788018092824,"score_spread":0.21564069882292897,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386742301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95719105,0.00015326925,0.04076933,0.000050725073,0.000015595906,0.000020672474,0.0004178209,0.0003556841,0.0010258671],"genre_scores_gemma":[0.9905539,0.000059675596,0.008958017,0.000012430329,0.000006073174,0.000010663988,0.00024798006,0.000020214782,0.00013106683],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99993527,0.000009893317,0.0000024796375,0.000019952713,0.000019844849,0.000012628621],"domain_scores_gemma":[0.99976283,0.00009713236,0.00005167484,0.000035966168,0.000018133142,0.000034218956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023651525,0.00025822004,0.00014503197,0.0005601616,0.00010207719,0.00023176397,0.00023415525,0.000360316,0.00070403283],"category_scores_gemma":[0.0005548148,0.00013261699,0.00016173846,0.00035688133,0.00015536277,0.00026337287,0.0003422962,0.000297411,0.0001455683],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048104534,0.00010534091,0.06942493,0.00013390646,0.00014541883,0.00035844318,0.00015592061,0.049594376,0.8384506,0.0018500525,0.00048682437,0.038813006],"study_design_scores_gemma":[0.00007012969,0.00045699024,0.24710727,0.000026662436,0.000083497864,0.00067373033,0.00013042611,0.5430099,0.20347959,0.0028521535,0.0020397832,0.00006983836],"about_ca_topic_score_codex":0.0006440796,"about_ca_topic_score_gemma":0.00055635127,"teacher_disagreement_score":0.00070403283,"about_ca_system_score_codex":0.00019004675,"about_ca_system_score_gemma":0.00011643382,"threshold_uncertainty_score":0.0023551583},"labels":[],"label_agreement":null},{"id":"W4386780215","doi":"10.3847/1538-4357/ace964","title":"Late-time Hubble Space Telescope Observations of AT 2018cow. II. Evolution of a UV-bright Underlying Source 2–4 Yr Post-discovery","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Astronomy; Luminosity; Brightness; Accretion (finance); Magnetar; Neutron star; Galaxy","score_opus":0.021874119507872228,"score_gpt":0.23784998602590898,"score_spread":0.21597586651803674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386780215","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99732363,0.000054533495,0.00017218142,0.000024478248,0.000008520823,0.00000679106,0.0012586043,0.000020165025,0.0011310173],"genre_scores_gemma":[0.99271953,0.00006368387,0.00035707952,0.0000149675225,0.00001687482,0.000013127905,0.004868198,0.000012530008,0.0019340647],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994814,0.000001833842,0.000002557885,0.00001250614,0.000012956371,0.000022065587],"domain_scores_gemma":[0.999603,0.000021708374,0.0001572215,0.00002971096,0.000061750405,0.0001267505],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000109877714,0.00024027102,0.00018537081,0.0010741143,0.00046002562,0.00042818193,0.0002190311,0.00022347708,0.0014643952],"category_scores_gemma":[0.0002271384,0.00009894249,0.00030276406,0.00054786034,0.00010170041,0.0002105921,0.0003972841,0.0002854507,0.0005586636],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003619021,0.00007165979,0.94743526,0.0000276261,0.00003364038,0.0013985181,0.00034684598,0.0002710082,0.037354533,0.00016672177,0.00084785547,0.011684404],"study_design_scores_gemma":[0.0000017587213,0.000014744312,0.9983246,0.0000019099718,0.000004392526,0.00009431037,0.000033287524,0.00007172141,0.0007735357,0.000012666273,0.00066524185,0.0000017976059],"about_ca_topic_score_codex":0.010163942,"about_ca_topic_score_gemma":0.019312795,"teacher_disagreement_score":0.010163942,"about_ca_system_score_codex":0.0005470127,"about_ca_system_score_gemma":0.00020082295,"threshold_uncertainty_score":0.02020955},"labels":[],"label_agreement":null},{"id":"W4386780246","doi":"10.3847/1538-4357/ace965","title":"Late-time Hubble Space Telescope Observations of AT 2018cow. I. Further Constraints on the Fading Prompt Emission and Thermal Properties 50–60 days Post-discovery","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Light curve; Luminosity; Blanketing; Photosphere; Hubble space telescope; RADIUS; Astronomy; Black-body radiation; Stars; Spectral line; Galaxy; Optics; Radiation","score_opus":0.024435914135898462,"score_gpt":0.21852382626419117,"score_spread":0.1940879121282927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386780246","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956328,0.000078331504,0.00033080316,0.00004103113,0.000015618029,0.000008252993,0.0022964033,0.000039678267,0.0015569851],"genre_scores_gemma":[0.9925655,0.00007363622,0.000356172,0.000022109225,0.000019997997,0.000019675757,0.0054893424,0.000025178904,0.0014284437],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999206,0.0000030862018,0.0000041212015,0.000019803798,0.000018442452,0.000033891916],"domain_scores_gemma":[0.99966764,0.0000134464735,0.00012375976,0.000034246837,0.000054682,0.0001061898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016006922,0.00025660807,0.00024387444,0.00088325114,0.0004397788,0.0005517803,0.00019718503,0.00020274865,0.0015992168],"category_scores_gemma":[0.0002474213,0.000116381976,0.00034886907,0.0006195395,0.00013719469,0.0002859661,0.0004432865,0.00029201663,0.0006636445],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007428026,0.00010603384,0.8960885,0.00006903861,0.00006212091,0.0010041994,0.00060003897,0.00069226016,0.07710714,0.00047134535,0.0026082185,0.020448355],"study_design_scores_gemma":[0.0000044366293,0.000020047035,0.99596393,0.000006000824,0.000009425293,0.000068199544,0.00006534743,0.0002135487,0.0012419528,0.000036423873,0.0023675049,0.0000031783813],"about_ca_topic_score_codex":0.011408563,"about_ca_topic_score_gemma":0.015534684,"teacher_disagreement_score":0.011408563,"about_ca_system_score_codex":0.0005437287,"about_ca_system_score_gemma":0.00026478688,"threshold_uncertainty_score":0.022684336},"labels":[],"label_agreement":null},{"id":"W4386833145","doi":"10.3847/1538-4357/acec3f","title":"Revisiting X-Ray-bright Optically Normal Galaxies with the Chandra Source Catalog","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Astrophysics; Active galactic nucleus; Quasar; Galaxy; QSOS; Redshift; Luminosity; Astronomy; Luminous infrared galaxy; Sky; Doubly ionized oxygen; Luminosity function; Radio galaxy; Emission spectrum; Spectral line","score_opus":0.006310679862324301,"score_gpt":0.19875578298392618,"score_spread":0.19244510312160187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386833145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.990515,0.00045137628,0.001800414,0.00007128847,0.000018014407,0.00007420007,0.0052721286,0.00011474874,0.0016826879],"genre_scores_gemma":[0.9825048,0.0003107605,0.0045820065,0.00006222725,0.000024381765,0.00006193766,0.011519252,0.000036527093,0.0008981971],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989629,0.00015806616,0.00018098902,0.00022384313,0.0002913235,0.00018288108],"domain_scores_gemma":[0.9941796,0.0009231141,0.0015572819,0.0018502143,0.0011014133,0.00038838637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017572279,0.00037381807,0.00029225004,0.006075037,0.00042269478,0.0012467853,0.00061941345,0.00020102256,0.0017447883],"category_scores_gemma":[0.006202497,0.00028496914,0.00033127138,0.00371314,0.00024913417,0.0008783018,0.0012127813,0.00024084878,0.0008694673],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048216454,0.00002003584,0.98629576,0.000028691094,0.000025484827,0.00006615085,0.00014091714,0.00021042256,0.001369279,0.00014762046,0.0008527268,0.010794563],"study_design_scores_gemma":[0.000004598832,0.000017000004,0.9932661,0.000022912425,0.00002166646,0.00016841164,0.00018412873,0.0010807129,0.000811004,0.00006692178,0.004350159,0.000006436992],"about_ca_topic_score_codex":0.036866352,"about_ca_topic_score_gemma":0.044322874,"teacher_disagreement_score":0.036866352,"about_ca_system_score_codex":0.00041950593,"about_ca_system_score_gemma":0.00062465336,"threshold_uncertainty_score":0.07330358},"labels":[],"label_agreement":null},{"id":"W4386907861","doi":"10.3847/1538-4357/ad31a5","title":"The Atacama Cosmology Telescope: Cosmology from Cross-correlations of unWISE Galaxies and ACT DR6 CMB Lensing","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":50,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"High Energy Physics; Office of Science; National Institute of Standards and Technology; Agencia Nacional de Investigación y Desarrollo; Nuclear Safety and Security Commission; Industry Canada; University of Toronto; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; National Research Foundation; Institut Périmètre de physique théorique; Flatiron Health; National Energy Research Scientific Computing Center; National Science Foundation; Compute Canada; National Aeronautics and Space Administration; Lawrence Berkeley National Laboratory; University of Pennsylvania; European Commission; U.S. Department of Energy; HORIZON EUROPE European Research Council; Princeton University; Government of Ontario; University of Cambridge; Ministry of Colleges and Universities; Government of Canada","keywords":"Physics","score_opus":0.008963047929049797,"score_gpt":0.243806878302784,"score_spread":0.23484383037373419,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386907861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97305995,0.0002148861,0.008825138,0.00019317382,0.000015104908,0.000012700299,0.0064017866,0.000462963,0.010814328],"genre_scores_gemma":[0.98863065,0.00006528804,0.0061448542,0.0000384073,0.000027938868,0.0000106053385,0.004203094,0.00017594988,0.0007032728],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99961853,0.000081939776,0.000015325522,0.000099743294,0.00015037865,0.000033986467],"domain_scores_gemma":[0.9971731,0.00052890426,0.0007635909,0.0007587267,0.0004851791,0.00029035896],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00092926103,0.00033084655,0.00025654543,0.0013044253,0.0003287334,0.00082468014,0.0004172406,0.00021325996,0.0022780297],"category_scores_gemma":[0.0032043883,0.00034822608,0.00040409435,0.0019443794,0.00040577006,0.000744341,0.00080958806,0.0006029038,0.0004782207],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036552158,0.000056720255,0.8878243,0.00011111421,0.00039395774,0.000294712,0.00091090053,0.026971763,0.022659555,0.009723892,0.009384319,0.041303165],"study_design_scores_gemma":[0.000006453234,0.000010403025,0.9771878,0.0000068989098,0.00001860068,0.00010488363,0.00005333264,0.0160158,0.0026875108,0.00083806453,0.0030514612,0.00001883211],"about_ca_topic_score_codex":0.019540802,"about_ca_topic_score_gemma":0.019508364,"teacher_disagreement_score":0.019540802,"about_ca_system_score_codex":0.0006949748,"about_ca_system_score_gemma":0.00023633357,"threshold_uncertainty_score":0.038854122},"labels":[],"label_agreement":null},{"id":"W4386915862","doi":"10.3847/1538-4357/aceb4a","title":"Are JWST/NIRCam Color Gradients in the Lensed z = 2.3 Dusty Star-forming Galaxy El Anzuelo Due to Central Dust Attenuation or Inside-out Galaxy Growth?","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; European Commission; National Natural Science Foundation of China; Goddard Space Flight Center; Chinese Academy of Sciences South America Center for Astronomy; Canadian Space Agency; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Attenuation; Star formation; Star (game theory); Cosmic dust; Optics","score_opus":0.01974909548053333,"score_gpt":0.2434296059785387,"score_spread":0.22368051049800536,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386915862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9971342,0.00005260684,0.00009095005,0.00007690169,0.0000046244004,0.000002651374,0.00039057396,0.00001995695,0.002227483],"genre_scores_gemma":[0.9985696,0.000025284895,0.0001609489,0.000038991482,0.000008254973,0.0000018727409,0.0006045766,0.000014812176,0.0005756198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991906,0.0000037529567,0.000002388764,0.000025583093,0.000019446821,0.000029727897],"domain_scores_gemma":[0.99973613,0.000017645816,0.00007705744,0.000025518622,0.00005443443,0.000089074776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014445436,0.00012376011,0.00015251857,0.0007778773,0.00023150668,0.0005866049,0.00026064602,0.00014317328,0.001745649],"category_scores_gemma":[0.00036049585,0.000108198954,0.00012627912,0.00038116562,0.00030423573,0.00027500812,0.00036915124,0.00014017931,0.000323937],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015689053,0.00002599454,0.9658734,0.000018154538,0.000041637515,0.00021090293,0.00045064467,0.00019619735,0.020908535,0.0005168288,0.0013334785,0.010267263],"study_design_scores_gemma":[0.000001725227,0.0000026701782,0.9990089,0.0000014691731,0.0000038871876,0.000022022714,0.00009201948,0.00017276309,0.00026050452,0.00003733016,0.0003946887,0.0000019107779],"about_ca_topic_score_codex":0.027556047,"about_ca_topic_score_gemma":0.04331078,"teacher_disagreement_score":0.027556047,"about_ca_system_score_codex":0.0005415252,"about_ca_system_score_gemma":0.00011344145,"threshold_uncertainty_score":0.05479133},"labels":[],"label_agreement":null},{"id":"W4386958902","doi":"10.3847/1538-4357/aced02","title":"Things That Might Go Bump in the Night: Assessing Structure in the Binary Black Hole Mass Spectrum","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Division of Astronomical Sciences; HORIZON EUROPE Marie Sklodowska-Curie Actions; Division of Physics; University of Oregon; H2020 European Research Council; National Aeronautics and Space Administration; Horizon 2020 Framework Programme; Space Telescope Science Institute; Division of Graduate Education; Villum Fonden; National Science Foundation","keywords":"Physics; Poisson distribution; Noise (video); Binary black hole; Binary number; Astrophysics; Statistical physics; Gravitational wave; Population; Spectral density; Black hole (networking); Statistics","score_opus":0.017433732383720958,"score_gpt":0.3180140843199712,"score_spread":0.3005803519362502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386958902","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99666697,0.000025159292,0.0018640192,0.000042193355,0.0000033501954,0.000017901231,0.00073068583,0.0001369778,0.000512784],"genre_scores_gemma":[0.9958248,0.000009996111,0.0025928596,0.000015711534,0.0000033069848,0.000011826482,0.0013742235,0.000032648328,0.00013467159],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996699,0.0001544209,0.000012036092,0.00006758751,0.00005991875,0.000036111705],"domain_scores_gemma":[0.99427587,0.004129739,0.00052949204,0.00045172672,0.00030147444,0.00031167225],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020653757,0.0002186282,0.00028539982,0.000712898,0.00031939262,0.00076058577,0.00060748996,0.000580506,0.0017216459],"category_scores_gemma":[0.00936399,0.00018388941,0.00042945324,0.0007003019,0.0005021536,0.0005733499,0.0006034462,0.0003967981,0.00017780361],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006275629,0.00030020752,0.73248816,0.00005214447,0.0002492651,0.0001430061,0.00037673712,0.24460435,0.0021014092,0.0028692044,0.0024473139,0.013740826],"study_design_scores_gemma":[0.0001252786,0.00032785063,0.34618247,0.000026349302,0.00007729283,0.00010633332,0.00028241382,0.6454021,0.002637257,0.0037511892,0.0010415972,0.000039959123],"about_ca_topic_score_codex":0.0067569287,"about_ca_topic_score_gemma":0.012124184,"teacher_disagreement_score":0.0067569287,"about_ca_system_score_codex":0.00054498564,"about_ca_system_score_gemma":0.0003642425,"threshold_uncertainty_score":0.013435185},"labels":[],"label_agreement":null},{"id":"W4386961147","doi":"10.3847/1538-4357/acec76","title":"The JWST Hubble Sequence: The Rest-frame Optical Evolution of Galaxy Structure at 1.5 &lt; z &lt; 6.5","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":108,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Royal Society; Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Star formation; Stellar mass; Universe; Galaxy formation and evolution; Stars","score_opus":0.009014103190420083,"score_gpt":0.22862587965129752,"score_spread":0.21961177646087743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4386961147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981818,0.00003242686,0.000089798785,0.000013899192,0.0000020294215,0.0000019877657,0.0011172001,0.00002128915,0.000539626],"genre_scores_gemma":[0.9973341,0.000013939295,0.00012681159,0.000005390508,0.0000035787089,0.0000016296431,0.0021027045,0.000007796435,0.00040401792],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.0000074571403,0.0000045358956,0.000031883577,0.000038978353,0.000039279494],"domain_scores_gemma":[0.9989876,0.000100097095,0.00034436595,0.000078542835,0.00016939176,0.0003199523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026824846,0.0001731336,0.00013724991,0.0016236332,0.00021498898,0.00054242375,0.00017142175,0.00018259055,0.0013007375],"category_scores_gemma":[0.00100804,0.00009873739,0.00021039884,0.00067239447,0.00017618602,0.000377594,0.0004235814,0.00021706417,0.00051630527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011155601,0.000033505632,0.98483723,0.000010844076,0.00005054218,0.000112897476,0.00018475877,0.00064039143,0.0074827946,0.00014085724,0.00090493134,0.0054896753],"study_design_scores_gemma":[6.3447175e-7,0.000005450261,0.99944454,6.730549e-7,0.0000020734458,0.0000151780405,0.00001573678,0.00023367337,0.00017489814,0.0000074216846,0.00009871102,9.359524e-7],"about_ca_topic_score_codex":0.013407841,"about_ca_topic_score_gemma":0.022795837,"teacher_disagreement_score":0.013407841,"about_ca_system_score_codex":0.00031601815,"about_ca_system_score_gemma":0.000108998516,"threshold_uncertainty_score":0.026659548},"labels":[],"label_agreement":null},{"id":"W4387045280","doi":"10.3847/1538-4357/ace434","title":"Evolutionary Origins of Binary Neutron Star Mergers: Effects of Common Envelope Efficiency and Metallicity","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Canadian Institute for Advanced Research; Northwestern University; Gordon and Betty Moore Foundation; University of Glasgow; Ford Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Common envelope; Neutron star; Metallicity; Mass ratio; Supernova; Binary number; Astronomy; White dwarf; Stars","score_opus":0.010597612299939099,"score_gpt":0.2989096557049303,"score_spread":0.28831204340499117,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387045280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990062,0.000051338127,0.00031038164,0.000026902604,0.000001909037,0.0000031884854,0.00005000814,0.00001126167,0.0005389084],"genre_scores_gemma":[0.99952984,0.00003022303,0.0002683982,0.0000065484737,0.0000012819902,0.000002267776,0.0000594261,0.000009952374,0.000092125956],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998485,0.000048413083,0.000011163238,0.000036208996,0.000022635577,0.00003306303],"domain_scores_gemma":[0.99910706,0.00045763742,0.0001621497,0.000068880705,0.00006941909,0.00013488348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008017401,0.00027868277,0.0003224405,0.00049304304,0.00045012162,0.0008671416,0.0004620798,0.00046932083,0.0010894799],"category_scores_gemma":[0.0030454986,0.00021333071,0.00037899488,0.00033852604,0.0005098617,0.0005222069,0.00059227116,0.00033607762,0.00012866326],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007376429,0.00022484535,0.6569868,0.00012840156,0.00025915256,0.00052029866,0.00044651088,0.28947148,0.032359555,0.009077334,0.0004879229,0.009300146],"study_design_scores_gemma":[0.00014492679,0.0003027074,0.29599422,0.00004309318,0.000111227586,0.00024325508,0.0004260858,0.6884119,0.00976723,0.0034024704,0.0011088809,0.00004409458],"about_ca_topic_score_codex":0.0040047434,"about_ca_topic_score_gemma":0.0037659022,"teacher_disagreement_score":0.0040047434,"about_ca_system_score_codex":0.00065071206,"about_ca_system_score_gemma":0.00026836948,"threshold_uncertainty_score":0.0079628825},"labels":[],"label_agreement":null},{"id":"W4387097684","doi":"10.3847/1538-4357/ace4bc","title":"Rapidly Evolving Transients in Archival ZTF Public Alerts","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"HORIZON EUROPE European Research Council; Israel Science Foundation; United States - Israel Binational Science Foundation","keywords":"Physics; Astrophysics; Transient (computer programming); Light curve; Astronomy; Kilonova; Gravitational wave; Event (particle physics); LIGO","score_opus":0.017920380520850928,"score_gpt":0.2395956047157791,"score_spread":0.22167522419492816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387097684","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9841568,0.0002897133,0.0008362044,0.00010145202,0.000019960116,0.00006186326,0.010943551,0.00018238145,0.0034079954],"genre_scores_gemma":[0.9693803,0.00023873133,0.0012481768,0.00006827991,0.000048443566,0.000062744824,0.026722444,0.00006598416,0.0021648605],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99929094,0.000043171214,0.00006830069,0.00012158323,0.00027101618,0.00020499989],"domain_scores_gemma":[0.996619,0.0005334022,0.0017274258,0.0003331994,0.00046479047,0.0003221672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009082897,0.00023482261,0.00023228185,0.0063890773,0.00047936395,0.0012571082,0.00048407374,0.00038364675,0.00410502],"category_scores_gemma":[0.0042765005,0.00013773105,0.0001705643,0.00493613,0.00025603376,0.00089854316,0.0011756221,0.00027324868,0.0011197863],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029809398,0.000048023743,0.95722383,0.000104654886,0.00003327136,0.00050618296,0.000669,0.00024989407,0.0029984831,0.0006084452,0.005617718,0.031642415],"study_design_scores_gemma":[0.0000088849665,0.000034802677,0.98786676,0.000043700362,0.000018517298,0.00038674066,0.00050665275,0.000719268,0.0012193947,0.00020339339,0.008979715,0.000012257595],"about_ca_topic_score_codex":0.015347215,"about_ca_topic_score_gemma":0.02540479,"teacher_disagreement_score":0.015347215,"about_ca_system_score_codex":0.000891972,"about_ca_system_score_gemma":0.0005589289,"threshold_uncertainty_score":0.03051579},"labels":[],"label_agreement":null},{"id":"W4387164952","doi":"10.3847/1538-4357/acf767","title":"Is a Recently Discovered H i Cloud near M94 a Starless Dark Matter Halo?","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"European Research Council; European Commission","keywords":"Physics; Astrophysics; Halo; Dark matter; Galaxy; Astronomy; Dark matter halo; Baryonic dark matter; Surface brightness","score_opus":0.01007181164364121,"score_gpt":0.22608258038310702,"score_spread":0.2160107687394658,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387164952","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989681,0.00013232812,0.000081873106,0.00007825495,0.0000054163274,0.0000035230164,0.00014263502,0.000011808737,0.000576177],"genre_scores_gemma":[0.9996313,0.00003763134,0.0000878164,0.000023199811,0.000014352734,9.589065e-7,0.00014307506,0.0000022485306,0.00005942295],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999002,0.000005142704,0.000005439533,0.000030248882,0.000024822559,0.000034138382],"domain_scores_gemma":[0.9996407,0.000028469924,0.0001250558,0.00003890405,0.000033111846,0.0001337455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013608343,0.00015595692,0.00025590003,0.0007736676,0.00088955695,0.0007809708,0.0006070944,0.0002942148,0.0010336767],"category_scores_gemma":[0.00048213915,0.0001540653,0.00014776122,0.0007165467,0.00049826864,0.00034577874,0.0006320288,0.0002890195,0.0002267941],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016963536,0.000041413048,0.9693226,0.000033259155,0.000079540165,0.005195383,0.0006228184,0.00019844453,0.01737757,0.0003268845,0.00064229994,0.0059901923],"study_design_scores_gemma":[0.000015252719,0.000055570115,0.9928966,0.000010625838,0.00003636347,0.0026150194,0.0007543019,0.0005445046,0.0009445631,0.00020922779,0.0019100662,0.00000792971],"about_ca_topic_score_codex":0.008285492,"about_ca_topic_score_gemma":0.008060142,"teacher_disagreement_score":0.008285492,"about_ca_system_score_codex":0.0006942962,"about_ca_system_score_gemma":0.00019424946,"threshold_uncertainty_score":0.016474545},"labels":[],"label_agreement":null},{"id":"W4387300677","doi":"10.3847/1538-4357/ace0c3","title":"Multimessenger Diagnostics of the Engine behind Core-collapse Supernovae","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Los Alamos National Laboratory; Aspen Center for Physics; U.S. Department of Energy; National Nuclear Security Administration; National Science Foundation","keywords":"Supernova; Physics; Astrophysics; Neutron star; Ejecta; Observable; Astronomy; Galaxy","score_opus":0.014876469780161314,"score_gpt":0.23979995603825818,"score_spread":0.22492348625809688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387300677","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98110664,0.00072058325,0.013005522,0.0001776866,0.000013796441,0.000024057772,0.0011843903,0.00043663091,0.0033307553],"genre_scores_gemma":[0.99705315,0.00015304693,0.0019721657,0.000019170802,0.000009404947,0.0000048363886,0.00056498504,0.00003256017,0.00019060228],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975723,0.0000798341,0.000019421028,0.00006438648,0.000046675697,0.00003244028],"domain_scores_gemma":[0.9979336,0.00065473694,0.00080834964,0.00031060094,0.00011159155,0.0001811137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014292941,0.00050669507,0.00032321084,0.0016092882,0.00024040298,0.0017643775,0.00058113487,0.0005392524,0.0013681289],"category_scores_gemma":[0.0039733513,0.00023562148,0.0004659018,0.0009893196,0.00040628057,0.0009898508,0.0011122645,0.0004434152,0.00033305516],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029592775,0.00010127212,0.88057274,0.00009782847,0.00039678576,0.0003358279,0.00025035036,0.06337091,0.011031417,0.017943071,0.00089118833,0.024712583],"study_design_scores_gemma":[0.000050335944,0.00014104188,0.69152564,0.00011278561,0.00012175743,0.00066240266,0.00033885526,0.26363647,0.0073783477,0.033100903,0.0028324935,0.00009890344],"about_ca_topic_score_codex":0.0037792516,"about_ca_topic_score_gemma":0.0043045287,"teacher_disagreement_score":0.0037792516,"about_ca_system_score_codex":0.00076385477,"about_ca_system_score_gemma":0.0003429639,"threshold_uncertainty_score":0.0075588822},"labels":[],"label_agreement":null},{"id":"W4387340354","doi":"10.3847/1538-4357/acf221","title":"A CHIME/FRB Study of Burst Rate and Morphological Evolution of the Periodically Repeating FRB 20180916B","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; York University; University of British Columbia; McGill University","funders":"Fonds de recherche du Québec – Nature et technologies; Institut Périmètre de physique théorique; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; National Research Council Canada; University of Toronto; Industry Canada; Canada Research Chairs; National Science Foundation; Government of Canada; Smithsonian Astrophysical Observatory; McGill University; Canadian Institute for Advanced Research","keywords":"Physics; Fast radio burst; Astrophysics; Phase (matter); Dispersion (optics); Binary number; Scattering; Variation (astronomy); Rotation period; Function (biology); Stars; Optics; Neutron star; Biology","score_opus":0.014172190339411164,"score_gpt":0.30414726743885595,"score_spread":0.2899750770994448,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387340354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99825853,0.00008306254,0.0002623935,0.000032448846,0.0000038363874,0.000005972677,0.0003687907,0.000030726875,0.00095424685],"genre_scores_gemma":[0.99828327,0.000037567086,0.00050445896,0.000015778029,0.000007142818,0.0000076198526,0.00080439093,0.00002166599,0.00031816357],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989724,0.0000073968463,0.000004960555,0.00003321245,0.00003061998,0.000026482205],"domain_scores_gemma":[0.9995776,0.00004846158,0.00012265792,0.000045543075,0.000082009356,0.00012381413],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002999513,0.00028369855,0.00028019867,0.0010171866,0.0004277146,0.0003889967,0.00031377378,0.00032805404,0.0009786558],"category_scores_gemma":[0.0006281216,0.0002165771,0.00025532098,0.0005665646,0.00022905636,0.0001776108,0.00033608178,0.00032502532,0.0003542038],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005422836,0.00007656908,0.7871298,0.000055270684,0.00012216302,0.0010400245,0.0006796845,0.0012819789,0.1904434,0.00029645723,0.0007524975,0.017579816],"study_design_scores_gemma":[0.0000070770952,0.00003523519,0.9963212,0.0000056036242,0.000011069885,0.00017059427,0.00007667135,0.0009529542,0.0016270637,0.000034598386,0.0007520378,0.000005858127],"about_ca_topic_score_codex":0.007304918,"about_ca_topic_score_gemma":0.009558817,"teacher_disagreement_score":0.007304918,"about_ca_system_score_codex":0.00037875702,"about_ca_system_score_gemma":0.00010963188,"threshold_uncertainty_score":0.014524758},"labels":[],"label_agreement":null},{"id":"W4387363825","doi":"10.3847/1538-4357/acf713","title":"Search for Extended Sources of Neutrino Emission in the Galactic Plane with IceCube","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Santen; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Compute Canada; Marquette University","keywords":"Physics; Neutrino; Galactic plane; Astrophysics; Cosmic ray; Galaxy; Astronomy; Muon; Neutrino astronomy; Neutrino detector; Neutrino oscillation; Nuclear physics","score_opus":0.015128598216834375,"score_gpt":0.2545834936125718,"score_spread":0.23945489539573744,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387363825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9815229,0.00042492355,0.0032912656,0.00011103319,0.000022997672,0.0000737372,0.006186465,0.00018825073,0.008178346],"genre_scores_gemma":[0.96958476,0.00033027976,0.010164857,0.00010265612,0.000053568376,0.00007964731,0.01850085,0.0000590648,0.0011243292],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997259,0.000058735204,0.00001109503,0.00007700257,0.000070640584,0.00005663159],"domain_scores_gemma":[0.99907887,0.00027216758,0.00025918527,0.00013949233,0.00011197433,0.00013830967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000775432,0.0002654471,0.00035924726,0.0010238902,0.00038273624,0.000755157,0.00034790637,0.00022638084,0.0013893633],"category_scores_gemma":[0.000730879,0.00015691607,0.0004043527,0.0015883717,0.00020773568,0.00025615975,0.00066832645,0.00029936936,0.0002459161],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0025382019,0.0003565186,0.8869604,0.00013589962,0.0007055226,0.0016677398,0.0005199735,0.014141402,0.048956934,0.0022271813,0.005511191,0.036279116],"study_design_scores_gemma":[0.00012443715,0.0003516315,0.9509299,0.00005809181,0.00020222041,0.0007651581,0.00033351308,0.014872943,0.012130686,0.0007792631,0.019428205,0.000023994065],"about_ca_topic_score_codex":0.0055134874,"about_ca_topic_score_gemma":0.010441602,"teacher_disagreement_score":0.0055134874,"about_ca_system_score_codex":0.0003909285,"about_ca_system_score_gemma":0.00038174217,"threshold_uncertainty_score":0.010962784},"labels":[],"label_agreement":null},{"id":"W4387368440","doi":"10.3847/1538-4357/ace34b","title":"Complex Organic Molecules in a Very Young Hot Corino, HOPS 373SW","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea","keywords":"Submillimeter Array; Protostar; Physics; Astrophysics; Millimeter; Sublimation (psychology); Opacity; Astrochemistry; Astronomy; Star formation; Stars; Galaxy; Interstellar medium; Optics","score_opus":0.01826824732632068,"score_gpt":0.24785094814451883,"score_spread":0.22958270081819815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387368440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.999432,0.000050710023,0.000033277924,0.0000061671317,0.0000014960042,0.0000022263732,0.000103111684,0.000007562609,0.00036327261],"genre_scores_gemma":[0.99925274,0.000031530348,0.00012997608,0.000011989778,0.0000033418155,0.0000019533522,0.00022915563,0.000004155733,0.00033510674],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99995756,0.0000011551498,0.0000015017135,0.000015753552,0.0000116352885,0.00001234444],"domain_scores_gemma":[0.9998958,0.000009807331,0.000029057883,0.0000068664986,0.000019146415,0.000039270948],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004791841,0.00028396267,0.00018408395,0.0007462722,0.0004822253,0.00028762306,0.0001873235,0.0002672032,0.0013800465],"category_scores_gemma":[0.0001036427,0.00012716872,0.00011579561,0.00045875963,0.00025692704,0.00017190806,0.00028009852,0.00015107694,0.00022814833],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044227333,0.000085836444,0.39417946,0.0000707528,0.000065323286,0.0051394883,0.0007989559,0.0001529526,0.5876168,0.0001444799,0.00043075063,0.0108728325],"study_design_scores_gemma":[0.000008884506,0.00015256801,0.97622603,0.00000578965,0.00002659673,0.0014402242,0.00066491315,0.00029918124,0.019444775,0.000050845218,0.0016714052,0.000008736977],"about_ca_topic_score_codex":0.004142414,"about_ca_topic_score_gemma":0.010066704,"teacher_disagreement_score":0.004142414,"about_ca_system_score_codex":0.00026225857,"about_ca_system_score_gemma":0.00009662564,"threshold_uncertainty_score":0.008236587},"labels":[],"label_agreement":null},{"id":"W4387368690","doi":"10.3847/1538-4357/aceef7","title":"The Green Bank North Celestial Cap Survey. VIII. 21 New Pulsar Timing Solutions","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia; McGill University","funders":"Office of Integrative Activities; National Science Foundation; European Research Council; U.S. Naval Research Laboratory; Natural Sciences and Engineering Research Council of Canada; Nederlandse Organisatie voor Wetenschappelijk Onderzoek","keywords":"Pulsar; Physics; Millisecond pulsar; Green Bank Telescope; Astrophysics; Binary pulsar; Astronomy; Pulsar planet; Accretion (finance); Orbit (dynamics)","score_opus":0.043020615256122725,"score_gpt":0.326809082811054,"score_spread":0.28378846755493126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387368690","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7085538,0.004406266,0.017015317,0.001701924,0.00080706464,0.00045696058,0.17224376,0.003625913,0.09118897],"genre_scores_gemma":[0.67635393,0.0020930655,0.045291435,0.00074863044,0.0006440815,0.00043013846,0.2567458,0.0006672773,0.017025724],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99942315,0.0000535491,0.00006516469,0.00011820299,0.00024026455,0.000099653626],"domain_scores_gemma":[0.99820185,0.00016485383,0.0005475401,0.000256101,0.00055284536,0.00027686337],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081161683,0.0005497657,0.00036473904,0.006948716,0.00053515885,0.0013622021,0.0005537663,0.0004724953,0.0061534145],"category_scores_gemma":[0.00213337,0.00027801242,0.0002825837,0.007638678,0.0002187241,0.0004988453,0.0008057949,0.0005713162,0.002731337],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047229108,0.00007502171,0.7008817,0.00030418555,0.00014062735,0.000745168,0.00072455197,0.0028996319,0.007895156,0.002663228,0.075767815,0.2074307],"study_design_scores_gemma":[0.00009155819,0.000071933275,0.8112258,0.00012679341,0.000063771186,0.00043442633,0.00032776964,0.0050498955,0.001836272,0.00079219934,0.17993516,0.00004456109],"about_ca_topic_score_codex":0.053181317,"about_ca_topic_score_gemma":0.103291415,"teacher_disagreement_score":0.053181317,"about_ca_system_score_codex":0.0013948998,"about_ca_system_score_gemma":0.0012375991,"threshold_uncertainty_score":0.10574353},"labels":[],"label_agreement":null},{"id":"W4387377478","doi":"10.3847/1538-4357/acf195","title":"VERTICO. VII. Environmental Quenching Caused by the Suppression of Molecular Gas Content and Star Formation Efficiency in Virgo Cluster Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Victoria; Royal Military College of Canada; McMaster University; Herzberg Institute of Astrophysics","funders":"National Research Foundation; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; Smithsonian Astrophysical Observatory; Australian Research Council; National Research Foundation of Korea; Agencia Nacional de Investigación y Desarrollo; Canada Research Chairs; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Virgo Cluster; Star formation; Galaxy; Quenching (fluorescence); Cluster (spacecraft); Galaxy cluster; Astronomy","score_opus":0.007288383711015675,"score_gpt":0.19740648164194444,"score_spread":0.19011809793092876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387377478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98937935,0.00027687475,0.0003181328,0.000040833187,0.00001393548,0.000007958528,0.00052086246,0.00006830066,0.009373794],"genre_scores_gemma":[0.99719703,0.0000745,0.00024898973,0.000012903572,0.000012323693,0.0000066378893,0.00058194663,0.000023782737,0.0018418232],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999126,0.000012857208,0.0000019676218,0.000031015275,0.000017849748,0.000023559065],"domain_scores_gemma":[0.9998983,0.000012011915,0.000023643199,0.000019186931,0.00001143233,0.00003545878],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000100753474,0.00014989128,0.0001964357,0.00038821282,0.00021790396,0.00051360804,0.00015419346,0.0001401805,0.0025471987],"category_scores_gemma":[0.00024074546,0.000071491515,0.00012660526,0.0003059437,0.00021567103,0.00010158981,0.00027553068,0.0001781573,0.00058047165],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015411717,0.00032794607,0.6130596,0.00019808438,0.00018390792,0.001781692,0.0011037107,0.00863214,0.2837668,0.0065291836,0.0047940905,0.07808169],"study_design_scores_gemma":[0.000015276142,0.00011668201,0.9823654,0.000011066405,0.000016403856,0.0002559596,0.00012371827,0.0039759018,0.0048485985,0.00046597066,0.0077969832,0.000007997468],"about_ca_topic_score_codex":0.005254383,"about_ca_topic_score_gemma":0.004406294,"teacher_disagreement_score":0.005254383,"about_ca_system_score_codex":0.00028220972,"about_ca_system_score_gemma":0.00008262407,"threshold_uncertainty_score":0.010447621},"labels":[],"label_agreement":null},{"id":"W4387409553","doi":"10.3847/1538-4357/acf46e","title":"Evolution of Planetary Obliquity: The Eccentric Kozai–Lidov Mechanism Coupled with Tide","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Natural Science Foundation of China","keywords":"Physics; Eccentricity (behavior); Angular momentum; Planet; Planetary system; Perturbation (astronomy); Kinetic energy; Astrophysics; Classical mechanics; Astronomy","score_opus":0.009376549313260048,"score_gpt":0.20765509257017098,"score_spread":0.19827854325691094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387409553","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913857,0.00013441399,0.0058117257,0.00020724194,0.000016143058,0.0000096591075,0.00008892741,0.00007553991,0.0022706236],"genre_scores_gemma":[0.9995197,0.000024043939,0.00025395982,0.000007261489,0.0000025821384,0.0000028455904,0.000015810563,0.0000077942905,0.0001659527],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991524,0.000024541248,0.0000052430587,0.000021484795,0.000012135599,0.00002134164],"domain_scores_gemma":[0.9994985,0.00012037593,0.0002092292,0.000031854375,0.00004488996,0.00009512345],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003382608,0.00029657682,0.00034077905,0.00054254377,0.00035734806,0.0005635932,0.0003868389,0.00036808592,0.00083406],"category_scores_gemma":[0.0017214959,0.00026498942,0.00038793054,0.00028638952,0.0005830937,0.000447111,0.0006566985,0.00034541913,0.000093218085],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034874713,0.000099164645,0.21737692,0.00017742731,0.00039509393,0.001360995,0.00045365957,0.66188824,0.075555675,0.028826999,0.0019302517,0.011586784],"study_design_scores_gemma":[0.000038973332,0.00005409033,0.07207962,0.000013587515,0.000038387258,0.00012437342,0.00006745712,0.92109454,0.0020895975,0.003918747,0.0004380287,0.000042622927],"about_ca_topic_score_codex":0.006346305,"about_ca_topic_score_gemma":0.002560424,"teacher_disagreement_score":0.006346305,"about_ca_system_score_codex":0.0007565377,"about_ca_system_score_gemma":0.00037888144,"threshold_uncertainty_score":0.01261878},"labels":[],"label_agreement":null},{"id":"W4387527738","doi":"10.3847/1538-4357/acef13","title":"First Results for Solar Soft X-Ray Irradiance Measurements from the Third-generation Miniature X-Ray Solar Spectrometer","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Heliophysics Division","keywords":"Physics; Solar flare; Solar maximum; Spectrometer; Flare; Solar cycle 22; Occultation; Coronal mass ejection; Solar irradiance; Satellite; Astronomy; Solar physics; Imaging spectrometer; Thermosphere; Astrophysics; Solar wind; Plasma; Ionosphere; Optics","score_opus":0.027487466792600296,"score_gpt":0.24225560993493467,"score_spread":0.21476814314233436,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387527738","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9761913,0.00025508256,0.006414668,0.000120012526,0.000050821494,0.00012776948,0.005117337,0.00078773504,0.010935308],"genre_scores_gemma":[0.97866154,0.00010291908,0.013259364,0.00010147975,0.000024528934,0.000058169084,0.0059958994,0.00011659991,0.0016795754],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99974126,0.000028072718,0.0000139854965,0.000053952255,0.00013767352,0.00002510662],"domain_scores_gemma":[0.9994722,0.00008609703,0.00004434039,0.00009124037,0.00021494628,0.00009122071],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076805725,0.00043752414,0.00029977006,0.00052690704,0.00054368936,0.0005780471,0.00032143993,0.00048236694,0.0021187651],"category_scores_gemma":[0.00042282479,0.00017470434,0.0004911302,0.00042213005,0.00016587865,0.00036169382,0.0004435306,0.00046377364,0.00057703455],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019048181,0.0008432053,0.51166266,0.00020186628,0.00037681265,0.0005213794,0.0005444846,0.004949858,0.40641376,0.000668883,0.006350084,0.065562114],"study_design_scores_gemma":[0.00011220896,0.0011024289,0.78099525,0.000017128492,0.00015026306,0.0003144323,0.00027899392,0.010347027,0.19539917,0.00020362703,0.011024426,0.00005509658],"about_ca_topic_score_codex":0.0021075036,"about_ca_topic_score_gemma":0.0063245543,"teacher_disagreement_score":0.0021187651,"about_ca_system_score_codex":0.00037478292,"about_ca_system_score_gemma":0.00021287292,"threshold_uncertainty_score":0.0070880055},"labels":[],"label_agreement":null},{"id":"W4387531510","doi":"10.3847/1538-4357/acf314","title":"Unraveling the Complexity of Dwarf Galaxy Dynamics: A Study of Binary Orbital Motions","year":2023,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Higher Education Discipline Innovation Project; National Natural Science Foundation of China; Natural Science Foundation of Shanghai","keywords":"Physics; Algorithm; Galaxy; Astrophysics; Computer science","score_opus":0.02665197065156407,"score_gpt":0.2513998339989709,"score_spread":0.22474786334740685,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387531510","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975178,0.00013811042,0.0016944527,0.00009206142,0.000004039053,0.0000027055023,0.00004663675,0.000021519774,0.00048267358],"genre_scores_gemma":[0.9991142,0.00005790093,0.0006681255,0.000008833558,0.0000052762075,0.0000015615698,0.0000493419,0.000009946092,0.00008476799],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998926,0.00003685998,0.0000068294084,0.000024553663,0.000017023762,0.00002211294],"domain_scores_gemma":[0.99857557,0.0007825017,0.0002687205,0.00014044455,0.00008073779,0.00015215161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005973687,0.0003033263,0.00047390108,0.00046935419,0.00044544466,0.00088414666,0.00038358822,0.0003633226,0.0008369313],"category_scores_gemma":[0.0033002226,0.00022304239,0.00044897164,0.00036511198,0.000512409,0.0009099919,0.0005671508,0.00046543108,0.00008014332],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030301354,0.00019695761,0.23321457,0.00010000992,0.00019138126,0.0004963946,0.0004264132,0.7322747,0.012574789,0.008930562,0.00050025043,0.010790981],"study_design_scores_gemma":[0.000011104307,0.00003596561,0.023808697,0.000006329102,0.000018642631,0.000029797804,0.00007754197,0.9739013,0.0007156545,0.0011957907,0.00019018477,0.00000905667],"about_ca_topic_score_codex":0.018340645,"about_ca_topic_score_gemma":0.007696248,"teacher_disagreement_score":0.018340645,"about_ca_system_score_codex":0.00044568424,"about_ca_system_score_gemma":0.00046264063,"threshold_uncertainty_score":0.03646779},"labels":[],"label_agreement":null},{"id":"W4387572911","doi":"10.3847/1538-4357/acf46f","title":"The Hubble Space Telescope Survey of M31 Satellite Galaxies. II. The Star Formation Histories of Ultrafaint Dwarf Galaxies","year":2023,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Nuclear Safety and Security Commission; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astronomy; Dwarf galaxy; Astrophysics; Hubble space telescope; Dwarf spheroidal galaxy; Galaxy; Elliptical galaxy; Luminous infrared galaxy; Hubble Deep Field; Galaxy group","score_opus":0.014701971536801861,"score_gpt":0.22265081254102856,"score_spread":0.2079488410042267,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387572911","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94810903,0.002064862,0.0007632148,0.00041351665,0.000018075898,0.000028218985,0.034915548,0.0002111543,0.01347636],"genre_scores_gemma":[0.97375995,0.00084978575,0.000609654,0.00008206482,0.00002593098,0.000020458703,0.018802447,0.00004011522,0.005809655],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998665,0.000014442239,0.000006715458,0.000033034,0.00003556819,0.000043817312],"domain_scores_gemma":[0.9989868,0.000108048036,0.00028498837,0.00017842384,0.0001951023,0.00024673663],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046363572,0.0002140624,0.00014039682,0.001491871,0.00031708076,0.00040017307,0.0002424008,0.00020854479,0.0029219908],"category_scores_gemma":[0.0012104299,0.0001258832,0.00017289766,0.0013485419,0.00017453184,0.00056593015,0.00042070274,0.00025930555,0.0013268585],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014617137,0.000026689308,0.9298852,0.00007803564,0.000040584404,0.00006573968,0.00060450606,0.00096469105,0.0018285917,0.0023255819,0.010646961,0.053387124],"study_design_scores_gemma":[0.000001999832,0.000009560029,0.9934041,0.000007409742,0.0000033572398,0.000024854831,0.000035477806,0.00023975615,0.00014665324,0.00016422254,0.0059600514,0.000002501822],"about_ca_topic_score_codex":0.061401024,"about_ca_topic_score_gemma":0.09649076,"teacher_disagreement_score":0.061401024,"about_ca_system_score_codex":0.0010584904,"about_ca_system_score_gemma":0.00037673375,"threshold_uncertainty_score":0.12208724},"labels":[],"label_agreement":null},{"id":"W4387578499","doi":"10.3847/1538-4357/acf201","title":"FORCASTing the Spectroscopic Dust Properties of the WC+O Binary WR 137 with SOFIA","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Embry-Riddle Aeronautical University; Universities Space Research Association; Research Corporation for Science Advancement","keywords":"Physics; Astrophysics; Circumstellar dust; Photometry (optics); Stars; Carbon star; Astronomy; Infrared; Spectral line; Cosmic dust; Emission spectrum; Circumbinary planet; Spectral energy distribution","score_opus":0.018944835463500707,"score_gpt":0.22569467130817794,"score_spread":0.20674983584467724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387578499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99924636,0.000010035202,0.00003537107,0.000004244538,0.0000016193012,0.0000022763445,0.00027987824,0.0000061003716,0.00041415863],"genre_scores_gemma":[0.9987717,0.00000568648,0.00010854742,0.0000039091774,0.00000162841,0.0000014731199,0.0009279504,0.0000037743314,0.00017527932],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998983,0.0000060376146,0.000007688094,0.000031165215,0.000027840226,0.00002899769],"domain_scores_gemma":[0.99980503,0.000017972225,0.000049065646,0.00003304284,0.00003845947,0.00005640134],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020290897,0.00020887153,0.00020805324,0.00051077886,0.0002646367,0.0003343372,0.00020542584,0.00014714693,0.0009899635],"category_scores_gemma":[0.00030377545,0.000094464325,0.00019752486,0.00035243796,0.000109132576,0.00019047852,0.00034242368,0.000150292,0.00022174956],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039054026,0.00008419398,0.9533827,0.000018030414,0.00009149181,0.00050915993,0.00025640507,0.0010942986,0.031345986,0.00009257153,0.000709576,0.012025134],"study_design_scores_gemma":[0.0000073799974,0.000050988947,0.9965185,0.0000018938783,0.000014042408,0.00006826362,0.00009370301,0.0009878816,0.00183554,0.000010516245,0.00040849435,0.0000026903758],"about_ca_topic_score_codex":0.018916408,"about_ca_topic_score_gemma":0.02656934,"teacher_disagreement_score":0.018916408,"about_ca_system_score_codex":0.0006628329,"about_ca_system_score_gemma":0.00016428427,"threshold_uncertainty_score":0.037612557},"labels":[],"label_agreement":null},{"id":"W4387614336","doi":"10.3847/1538-4357/ace599","title":"The Atacama Cosmology Telescope: Systematic Transient Search of 3 Day Maps","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Agencia Nacional de Investigación y Desarrollo; University of Toronto; Science and Technology Facilities Council; European Commission; University of Pennsylvania; Princeton University; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Sky; Astronomy; Telescope; Stars; Cosmology; Variable star; Flare; Transient (computer programming)","score_opus":0.012717725515747241,"score_gpt":0.24189478416906005,"score_spread":0.2291770586533128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387614336","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9672605,0.00039629312,0.013317669,0.000051470255,0.000014115268,0.00017532603,0.014246425,0.0009790041,0.0035592257],"genre_scores_gemma":[0.94772226,0.00013805288,0.025712183,0.000049833397,0.000021213578,0.00014489233,0.0251275,0.00024473807,0.0008393558],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99932885,0.00010506758,0.000067084846,0.0001916391,0.00020661576,0.00010079621],"domain_scores_gemma":[0.9956487,0.0006797115,0.0011883901,0.0011883674,0.0009056655,0.0003891504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014363711,0.00024230123,0.00039241195,0.004960244,0.0010185048,0.0009652522,0.00062913407,0.00030947517,0.0012772395],"category_scores_gemma":[0.0024911857,0.00026346833,0.0004969477,0.005899223,0.00028703792,0.00038885712,0.0008458581,0.0002910885,0.00070460775],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046155995,0.00013553734,0.8797903,0.00018813065,0.0003460234,0.0008701769,0.0010438181,0.0025351273,0.04133973,0.00088553905,0.0070394864,0.065364495],"study_design_scores_gemma":[0.000018042925,0.000050256418,0.98606133,0.000012497076,0.00005919061,0.00034983814,0.00020009285,0.0041314145,0.0034715792,0.00022078582,0.0054071643,0.000017852493],"about_ca_topic_score_codex":0.013607618,"about_ca_topic_score_gemma":0.027744966,"teacher_disagreement_score":0.013607618,"about_ca_system_score_codex":0.0005876886,"about_ca_system_score_gemma":0.0013892793,"threshold_uncertainty_score":0.027056813},"labels":[],"label_agreement":null},{"id":"W4387614940","doi":"10.3847/1538-4357/acf46b","title":"The High-redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Investigating the Role of Environment on Bent Radio AGNs Using LOFAR","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; National Key Research and Development Program of China; Jet Propulsion Laboratory; Office of Science; Centre National de la Recherche Scientifique; Brookhaven National Laboratory; Northern Arizona University; Tsinghua University; Harvard University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; U.S. Department of Energy; National Natural Science Foundation of China; York University; Carnegie Mellon University; University of Arizona; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; University of Toledo; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; California Institute of Technology; National Aeronautics and Space Administration","keywords":"LOFAR; Physics; Astrophysics; Bent molecular geometry; Spectral index; Redshift; Active galactic nucleus; Sky; Cluster (spacecraft); Astronomy; Luminosity; Radio telescope; Spectral line; Galaxy","score_opus":0.013185597298083327,"score_gpt":0.21260458889323103,"score_spread":0.1994189915951477,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387614940","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99917895,0.00002241322,0.00012524372,0.000012468069,6.440701e-7,0.0000017796002,0.00028030173,0.000010294523,0.0003679061],"genre_scores_gemma":[0.99887866,0.000013383786,0.00016648632,0.000012379619,0.0000036420386,0.0000021679725,0.0007672151,0.000006308911,0.00014965913],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999749,0.000046282326,0.000011388871,0.000076932054,0.0000479296,0.0000684588],"domain_scores_gemma":[0.9987972,0.00016616458,0.00048514735,0.00014657623,0.00011254038,0.00029229946],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033987433,0.00017292173,0.00018781998,0.0009785626,0.00032088175,0.00066059193,0.00024239477,0.00015424391,0.0010880163],"category_scores_gemma":[0.00079106103,0.0001569557,0.00017972768,0.0005579909,0.0003300728,0.00030468416,0.00067810225,0.0001950795,0.0002920715],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006885563,0.000016671742,0.9928677,0.00000707043,0.00003370991,0.000046171568,0.0001336489,0.00024114708,0.00438145,0.0000826002,0.00022070287,0.0019002876],"study_design_scores_gemma":[0.0000011657468,0.0000078779485,0.9995889,7.45543e-7,0.0000040222726,0.0000177598,0.00005440047,0.00015051753,0.00008391772,0.00000780267,0.0000815055,0.000001286572],"about_ca_topic_score_codex":0.0062445486,"about_ca_topic_score_gemma":0.0147794,"teacher_disagreement_score":0.0062445486,"about_ca_system_score_codex":0.00021518441,"about_ca_system_score_gemma":0.00012103347,"threshold_uncertainty_score":0.012416363},"labels":[],"label_agreement":null},{"id":"W4387779949","doi":"10.3847/1538-4357/acf3e8","title":"The Panchromatic Hubble Andromeda Treasury: Triangulum Extended Region (PHATTER). V. The Structure of M33 in Resolved Stellar Populations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Local Group; Halo; Andromeda; Stellar mass; Spiral galaxy; Galaxy; Stellar population; Star formation; Milky Way","score_opus":0.016051701234076288,"score_gpt":0.23766840320047433,"score_spread":0.22161670196639804,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387779949","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9839669,0.0003198525,0.0023483024,0.000052407402,0.000007501263,0.000034191242,0.006277435,0.00024363211,0.0067498274],"genre_scores_gemma":[0.98858976,0.000089399226,0.0048686797,0.000022713653,0.0000126874775,0.000019818797,0.004749975,0.00005256331,0.0015943734],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984217,0.000021382353,0.000004323028,0.00004942968,0.00003337471,0.00004933389],"domain_scores_gemma":[0.9995734,0.000038979193,0.0001704629,0.00008643889,0.000057034133,0.00007359785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024219172,0.00022557222,0.00013132075,0.0014038447,0.00021960428,0.00033880028,0.00031756266,0.00020609189,0.0023101268],"category_scores_gemma":[0.0006209497,0.00010354234,0.00027605315,0.0011350374,0.00010144799,0.00024495996,0.00042196005,0.00016591314,0.00084927434],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002445125,0.000030442161,0.8803384,0.000071220464,0.00015690821,0.0005965128,0.00034502283,0.0023080022,0.03620388,0.00087901985,0.0046216315,0.07420448],"study_design_scores_gemma":[0.0000030792442,0.000019595234,0.993359,0.00000645586,0.000009137449,0.00023814762,0.000040155923,0.0014172356,0.0009779107,0.000056003722,0.0038658993,0.000007445688],"about_ca_topic_score_codex":0.018234326,"about_ca_topic_score_gemma":0.028297797,"teacher_disagreement_score":0.018234326,"about_ca_system_score_codex":0.0002698782,"about_ca_system_score_gemma":0.00013564127,"threshold_uncertainty_score":0.036256373},"labels":[],"label_agreement":null},{"id":"W4387783899","doi":"10.3847/1538-4357/acefcf","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): The Warm-envelope Origin of Hot Corinos","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Key Research and Development Program of China; Ministry of Science and ICT, South Korea; National Research Foundation of Korea; Academy of Finland; National Natural Science Foundation of China; Chinese Academy of Sciences; Japan Society for the Promotion of Science; Agencia Nacional de Investigación y Desarrollo; Ministry of Education, Culture, Sports, Science and Technology","keywords":"Physics; Astrophysics; Young stellar object; Protostar; Submillimeter Array; Astronomy; Luminosity; Spectral energy distribution; Molecular cloud; Star formation; Stars; Galaxy","score_opus":0.032685328103406956,"score_gpt":0.27372859265656285,"score_spread":0.2410432645531559,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387783899","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99871325,0.00008934614,0.00019522902,0.000016856,0.0000013473442,0.000004096957,0.0005236441,0.000016368931,0.00043988533],"genre_scores_gemma":[0.9989498,0.000045839522,0.00023635746,0.0000083098785,0.000003560521,0.0000034241164,0.000607646,0.00000468424,0.00014040303],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990773,0.000012543449,0.0000038011701,0.00003684704,0.000017813305,0.000021312437],"domain_scores_gemma":[0.9997181,0.000036273188,0.00011225722,0.000039239712,0.000030037794,0.000063991945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025937628,0.00020005029,0.00012384074,0.000749949,0.00026917743,0.00038558195,0.00024404962,0.00011629456,0.0008153687],"category_scores_gemma":[0.0003583379,0.00008239425,0.0001783422,0.00047966742,0.00013435607,0.00023475187,0.0004206243,0.0001053328,0.00022550812],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000067597015,0.000017721264,0.9847718,0.000024398223,0.000042915966,0.00008914437,0.00018403446,0.00049755414,0.006755452,0.0002295314,0.0003955663,0.00692412],"study_design_scores_gemma":[0.000002814469,0.000015151239,0.9967372,0.0000052878304,0.000014431266,0.000051776653,0.0001344699,0.0016048832,0.0007608853,0.00006165622,0.0006085971,0.000002790687],"about_ca_topic_score_codex":0.0072042234,"about_ca_topic_score_gemma":0.0069143996,"teacher_disagreement_score":0.0072042234,"about_ca_system_score_codex":0.00027970143,"about_ca_system_score_gemma":0.00014433719,"threshold_uncertainty_score":0.014324605},"labels":[],"label_agreement":null},{"id":"W4387875382","doi":"10.3847/1538-4357/acfa02","title":"The Polarized Cosmic Hand: IXPE Observations of PSR B1509−58/MSH 15−5<sup>2</sup>","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"NASA Headquarters; Marshall Space Flight Center; Agenzia Spaziale Italiana","keywords":"Physics; Polarization (electrochemistry); Astrophysics; Pulsar; Magnetic field; Linear polarization; Nebula; Brewster's angle; Astronomy; Optics; Stars; Laser","score_opus":0.025315957219115146,"score_gpt":0.3145864232824531,"score_spread":0.28927046606333795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387875382","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99162465,0.0001280144,0.00052841567,0.000044929955,0.000008482772,0.000008410074,0.00080880517,0.00005948683,0.006788872],"genre_scores_gemma":[0.9977175,0.00007850345,0.00072346744,0.000053319127,0.000022523125,0.0000051780416,0.00084263127,0.000013679374,0.00054333254],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996316,0.0000024768847,0.0000014331526,0.000011443728,0.000010959307,0.000010505612],"domain_scores_gemma":[0.9999051,0.000012799087,0.000027485508,0.0000136221015,0.0000123757,0.000028571956],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008622787,0.00017145526,0.00011613486,0.0005617681,0.00022639055,0.00030385598,0.00011201405,0.00015273076,0.0014270548],"category_scores_gemma":[0.00016884471,0.000114893046,0.00008591688,0.00034126852,0.00013234223,0.00014734843,0.0002922183,0.00018294012,0.00025826483],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001164357,0.00012897929,0.5622171,0.000096468444,0.00015733487,0.0020601586,0.00039449782,0.0010872384,0.36702,0.0011882015,0.0036024156,0.06088319],"study_design_scores_gemma":[0.000019766545,0.00005819632,0.9858349,0.000013021987,0.000028746885,0.0007456506,0.000058577127,0.00057669054,0.009685269,0.00019489523,0.0027789436,0.0000054577577],"about_ca_topic_score_codex":0.0009788218,"about_ca_topic_score_gemma":0.003664396,"teacher_disagreement_score":0.0014270548,"about_ca_system_score_codex":0.000147525,"about_ca_system_score_gemma":0.00006499178,"threshold_uncertainty_score":0.0047739744},"labels":[],"label_agreement":null},{"id":"W4387880037","doi":"10.3847/1538-4357/acef18","title":"A Comprehensive Optical Search for Pre-explosion Outbursts from the Quiescent Progenitor of SN 2023ixf","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Deutsches Elektronen-Synchrotron; Stockholms Universitet; Institut National de Physique Nucléaire et de Physique des Particules; California Institute of Technology; Trinity College Dublin; John Templeton Foundation; Heising-Simons Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Light curve; Brightness; Supergiant; Astronomy; Stars; Red supergiant","score_opus":0.03208350065726089,"score_gpt":0.29320850638240475,"score_spread":0.26112500572514385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387880037","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976119,0.00018239008,0.0003694291,0.000012927728,0.0000014920996,0.000012123935,0.0008855376,0.000036758367,0.0008873776],"genre_scores_gemma":[0.9949923,0.00012012385,0.0010901418,0.000023866627,0.0000054600287,0.000010090906,0.003523438,0.0000074758896,0.00022708534],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991167,0.0000061645446,0.000004740144,0.000016743887,0.0000266649,0.00003394632],"domain_scores_gemma":[0.99956053,0.00006200028,0.00014558517,0.000026600026,0.00006365474,0.00014161854],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033721744,0.0002908688,0.00024394329,0.0019780912,0.00047735422,0.00039808272,0.00023773726,0.0002579142,0.00094276195],"category_scores_gemma":[0.0003489108,0.00014886119,0.00034718754,0.0009018664,0.0001121129,0.00020038511,0.0003544154,0.00013523409,0.00023309073],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017643221,0.00006507126,0.9568352,0.0000417012,0.00006464262,0.0006381988,0.00013868384,0.00039429622,0.026838116,0.000116579424,0.0003745153,0.014316524],"study_design_scores_gemma":[0.000004427795,0.000093678376,0.99440837,0.000007014584,0.000028539274,0.0005403882,0.00011300578,0.0007802732,0.0028298907,0.00005942675,0.0011284805,0.000006630984],"about_ca_topic_score_codex":0.008974862,"about_ca_topic_score_gemma":0.016672393,"teacher_disagreement_score":0.008974862,"about_ca_system_score_codex":0.00032321486,"about_ca_system_score_gemma":0.00033837097,"threshold_uncertainty_score":0.017845213},"labels":[],"label_agreement":null},{"id":"W4387882108","doi":"10.3847/1538-4357/accea2","title":"FAST-ASKAP Synergy: Quantifying Coexistent Tidal and Ram Pressure Strippings in the NGC 4636 Group","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"SLAC National Accelerator Laboratory; High Energy Physics; Division of Astronomical Sciences; Agencia Estatal de Investigación; European Regional Development Fund; Leibniz-Gemeinschaft; York University; Ministério da Ciência, Tecnologia e Inovação; Science and Technology Facilities Council; Office of Science; University of Colorado Boulder; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Korea Astronomy and Space Science Institute; Ministry of Science and Technology of the People's Republic of China; Centre National d’Etudes Spatiales; Chinese Academy of Sciences; Peking University; Commonwealth Scientific and Industrial Research Organisation; University of Sussex; University of Nottingham; European Commission; University of Oxford; National Energy Research Scientific Computing Center; Australian Government; Science and Industry Endowment Fund; National Science Foundation; University of Michigan; University of Notre Dame; Bundesministerium für Bildung und Forschung; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Portsmouth; New Mexico State University; University of Utah; National Natural Science Foundation of China; Ohio State University; University of California; Yale University; Government of Western Australia; U.S. Department of Energy; Smithsonian Institution; Ministry of Science and ICT, South Korea; University of Pennsylvania; National Aeronautics and Space Administration; National Astronomical Observatories, Chinese Academy of Sciences; California Institute of Technology; Vanderbilt University","keywords":"Physics; Astrophysics; Stripping (fiber); Galaxy; Ram pressure; Telescope; Sky; Astronomy; Star formation","score_opus":0.018464171142698573,"score_gpt":0.2430199749352669,"score_spread":0.22455580379256831,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387882108","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99841344,0.000038981816,0.00025389876,0.0000146027705,0.0000012425915,0.000006070783,0.00090200285,0.000038423455,0.00033137354],"genre_scores_gemma":[0.9977156,0.000020882499,0.0007711946,0.000008487643,0.000004079724,0.000008918502,0.0012539654,0.000007969024,0.00020892688],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955434,0.00008336278,0.000030436573,0.00012945545,0.00011871629,0.000083738225],"domain_scores_gemma":[0.9986009,0.000126781,0.00044699153,0.000273401,0.00016827579,0.0003836463],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00079026463,0.00035664972,0.00037659353,0.0023860661,0.00037857582,0.0005620768,0.00044821287,0.00032000954,0.0006800921],"category_scores_gemma":[0.0014981235,0.0002023948,0.00043740883,0.0016227206,0.000283305,0.0005274332,0.0010067208,0.00018420353,0.000371988],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000080229365,0.000019224002,0.98852056,0.0000185251,0.000085885935,0.00006118331,0.00039369686,0.00063129724,0.004828503,0.00005147564,0.00021500427,0.0050944174],"study_design_scores_gemma":[0.0000016685574,0.000019074208,0.9982741,0.0000020761197,0.000015525507,0.000040465908,0.00013896626,0.0008613196,0.0003672863,0.000025632096,0.00025010874,0.0000037253335],"about_ca_topic_score_codex":0.025868922,"about_ca_topic_score_gemma":0.028945982,"teacher_disagreement_score":0.025868922,"about_ca_system_score_codex":0.0004620331,"about_ca_system_score_gemma":0.00031716024,"threshold_uncertainty_score":0.051436722},"labels":[],"label_agreement":null},{"id":"W4387974995","doi":"10.3847/1538-4357/acf3e6","title":"Magnetic Structures and Turbulence in SN 1006 Revealed with Imaging X-Ray Polarimetry","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Smithsonian Astrophysical Observatory; Istituto Nazionale di Fisica Nucleare; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Goddard Space Flight Center; Smithsonian Institution; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Hong Kong Government; National Natural Science Foundation of China; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Polarization (electrochemistry); Astrophysics; Magnetic field; Supernova; Polarimetry; Particle acceleration; Sky; Degree of polarization; Cosmic ray; Supernova remnant; Astronomy; Optics; Scattering","score_opus":0.004304882452130068,"score_gpt":0.2066009850147125,"score_spread":0.20229610256258243,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4387974995","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99903727,0.000035709414,0.00023244883,0.0000095511,0.0000021289386,0.0000028992881,0.00013096063,0.000016028953,0.0005331176],"genre_scores_gemma":[0.99914765,0.00003274646,0.00037035646,0.0000056563676,0.0000044966846,0.0000018584698,0.0002916946,0.0000054038283,0.00014020201],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999559,0.000004508045,0.0000028345682,0.000012021454,0.000014758576,0.000009968207],"domain_scores_gemma":[0.9998567,0.0000108822915,0.000052359137,0.000014706479,0.000024900693,0.00004043848],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000116082614,0.00022822383,0.00016755654,0.00095414603,0.000201569,0.0003913062,0.00013570285,0.00016536635,0.0005930269],"category_scores_gemma":[0.00020310737,0.00015564673,0.00016766314,0.0005490101,0.00023372454,0.00017755796,0.00050873787,0.00020157399,0.00014028094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005745593,0.00008048608,0.7141086,0.000034757457,0.00008107327,0.0019201263,0.0002976438,0.0014688775,0.2710228,0.00040455107,0.00034755585,0.009658967],"study_design_scores_gemma":[0.00001135489,0.000051863695,0.9919932,0.000004326736,0.000013349061,0.0005965235,0.00011470942,0.0022203447,0.0044662105,0.00011354994,0.00040494604,0.000009632673],"about_ca_topic_score_codex":0.0021716552,"about_ca_topic_score_gemma":0.0025536146,"teacher_disagreement_score":0.0021716552,"about_ca_system_score_codex":0.00011568746,"about_ca_system_score_gemma":0.00007343207,"threshold_uncertainty_score":0.004317999},"labels":[],"label_agreement":null},{"id":"W4388021565","doi":"10.3847/1538-4357/ace971","title":"Needle in a Haystack: Finding Supermassive Black Hole-related Flares in the Zwicky Transient Facility Public Survey","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"HORIZON EUROPE European Research Council; Israel Science Foundation; United States - Israel Binational Science Foundation; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Supermassive black hole; Astrophysics; Galaxy; Supernova; Astronomy; Active galactic nucleus; Population; Black hole (networking); Redshift","score_opus":0.02529729881451238,"score_gpt":0.23823809943589444,"score_spread":0.21294080062138207,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388021565","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9898846,0.00017191534,0.00053967594,0.0001766982,0.0000052513205,0.00006323821,0.00795855,0.00012592057,0.001074055],"genre_scores_gemma":[0.98282284,0.0002128011,0.0022231906,0.00016595915,0.00001620075,0.000043963184,0.013379007,0.00004937764,0.0010868127],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99956506,0.00004613162,0.000033731663,0.00012293966,0.0001039839,0.00012815378],"domain_scores_gemma":[0.9984921,0.00031479483,0.00064385857,0.0001234034,0.00017954335,0.00024629102],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000604652,0.0002061595,0.00016640635,0.0031540662,0.00046541024,0.0006688671,0.00049791567,0.00026829145,0.0029317276],"category_scores_gemma":[0.0024009163,0.000113798334,0.0001958567,0.0018552437,0.00024780634,0.00073362945,0.001023252,0.00022659419,0.0005749234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000077743454,0.00003189937,0.9796545,0.000045752036,0.000037247046,0.00031901943,0.00042567658,0.00013988206,0.0021719912,0.00010510437,0.003809826,0.013181401],"study_design_scores_gemma":[0.000014355819,0.000072085604,0.98926216,0.000054386972,0.00003365775,0.0005844057,0.0019746656,0.0015303319,0.00140792,0.00011437311,0.0049368474,0.000014804193],"about_ca_topic_score_codex":0.04838205,"about_ca_topic_score_gemma":0.08988293,"teacher_disagreement_score":0.04838205,"about_ca_system_score_codex":0.00069346966,"about_ca_system_score_gemma":0.000642918,"threshold_uncertainty_score":0.09620088},"labels":[],"label_agreement":null},{"id":"W4388023724","doi":"10.3847/1538-4357/acfe11","title":"Turbulent Structure in Supernova Remnants G46.8−0.3 and G39.2−0.3 from THOR Polarimetry","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Faraday effect; Astrophysics; Interstellar medium; Supernova; Polarization (electrochemistry); Faraday cage; Supernova remnant; Polarimetry; Linear polarization; Astronomy; Optics; Magnetic field; Galaxy; Scattering","score_opus":0.008825884762332162,"score_gpt":0.22940645024873627,"score_spread":0.2205805654864041,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388023724","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995004,0.000032634416,0.00006658804,0.0000037731895,6.9055574e-7,9.0014015e-7,0.00014388672,0.000005356512,0.00024584174],"genre_scores_gemma":[0.99927217,0.000031102925,0.0000678682,0.0000037185816,0.000002332717,9.1744613e-7,0.0005499027,0.0000037796126,0.0000681965],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.000008085545,0.0000051258726,0.000016785432,0.00001621412,0.000016863733],"domain_scores_gemma":[0.9996228,0.000037274596,0.00017523958,0.000038480346,0.00004493384,0.00008114917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019994615,0.00016371443,0.00016074357,0.000927377,0.0001982613,0.0004984796,0.0001148558,0.00009685469,0.00067917234],"category_scores_gemma":[0.000395764,0.00009783391,0.00021519755,0.0006124241,0.00028693065,0.0001588092,0.00044964795,0.00010505304,0.00022263468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022081526,0.000016368496,0.9695995,0.000013706723,0.0000593311,0.00019065278,0.00035632472,0.00045851586,0.025300145,0.00016659347,0.000099537676,0.003518555],"study_design_scores_gemma":[0.0000014792034,0.000010723431,0.9991008,0.0000012116981,0.0000066229727,0.000054986525,0.000057337416,0.00017685286,0.00043820165,0.000025456457,0.00012425627,0.0000022261195],"about_ca_topic_score_codex":0.0039936607,"about_ca_topic_score_gemma":0.003823523,"teacher_disagreement_score":0.0039936607,"about_ca_system_score_codex":0.00015866087,"about_ca_system_score_gemma":0.00006134447,"threshold_uncertainty_score":0.007940829},"labels":[],"label_agreement":null},{"id":"W4388079984","doi":"10.3847/1538-4357/acfe0e","title":"Beyond the Drake Equation: A Time-dependent Inventory of Habitable Planets and Life-bearing Worlds in the Solar Neighborhood","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Nuclear Safety and Security Commission; New York University Abu Dhabi; York University; National Aeronautics and Space Administration","keywords":"Exoplanet; Planet; Circumstellar habitable zone; Astrobiology; Terrestrial planet; Solar System; Astronomy; Physics; Population; Planetary habitability; Metallicity; Stars; Astrophysics; Demography","score_opus":0.015017886549249107,"score_gpt":0.21984348575371626,"score_spread":0.20482559920446716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388079984","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.44943082,0.0017068344,0.50517327,0.0068547,0.0001677181,0.0001507359,0.0025826783,0.00021306172,0.033720143],"genre_scores_gemma":[0.93241906,0.0013848296,0.042108193,0.00044579533,0.0002546959,0.00028205014,0.0008533364,0.000101867336,0.022150185],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991936,0.0001701917,0.000042674066,0.0002636192,0.00015605267,0.0001739443],"domain_scores_gemma":[0.9935521,0.0029124422,0.0015542804,0.00042540926,0.0007147511,0.00084098516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022381574,0.000480229,0.0011482801,0.0022879457,0.0011299385,0.002749793,0.0020169194,0.0011063975,0.007858234],"category_scores_gemma":[0.012472931,0.00046205337,0.0013544899,0.0012467139,0.0022524612,0.0093336245,0.0030876554,0.0023072471,0.0008216336],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004059455,0.00004954905,0.033880167,0.00006371794,0.000060813993,0.0003750181,0.00056154357,0.07345401,0.0007766466,0.8788659,0.003202667,0.008669413],"study_design_scores_gemma":[0.000016012522,0.000037103306,0.007524369,0.0000328797,0.000033987013,0.0003329319,0.00037696926,0.60726494,0.00023462066,0.3780569,0.0060360534,0.000053236952],"about_ca_topic_score_codex":0.012903353,"about_ca_topic_score_gemma":0.005880673,"teacher_disagreement_score":0.012903353,"about_ca_system_score_codex":0.0013673453,"about_ca_system_score_gemma":0.0011779048,"threshold_uncertainty_score":0.02628845},"labels":[],"label_agreement":null},{"id":"W4388131621","doi":"10.3847/1538-4357/acfa96","title":"GTC Follow-up Observations of Very Metal-poor Star Candidates from DESI","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Horizon 2020 Framework Programme; Office of Science; Division of Astronomical Sciences; Instituto de Astrofísica de Canarias; Ministerio de Ciencia e Innovación; Gordon and Betty Moore Foundation; U.S. Department of Energy; National Science Foundation","keywords":"Stars; Milky Way; Astrophysics; Physics; Astronomy; Spectroscopy; Spectral line","score_opus":0.02862104218947141,"score_gpt":0.2371464552707219,"score_spread":0.2085254130812505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388131621","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9901484,0.00010939913,0.0008991215,0.00007980891,0.000016427286,0.00003641475,0.0044852523,0.00015240029,0.004072654],"genre_scores_gemma":[0.98127055,0.000065530105,0.0027649247,0.00012964534,0.000031174288,0.000033555345,0.012698444,0.00010825396,0.0028978856],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997011,0.00002564175,0.000008354482,0.00010312322,0.00009151148,0.000070294685],"domain_scores_gemma":[0.9990565,0.00006577314,0.00017478039,0.00015969214,0.00027855052,0.00026459017],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052932784,0.0003456252,0.00035096033,0.0014780156,0.0006467162,0.00046018985,0.0003360366,0.00038347123,0.0013417355],"category_scores_gemma":[0.000558419,0.00018275513,0.00030523978,0.00096448197,0.00024894896,0.00019084428,0.00073050545,0.00039431278,0.001026213],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007426012,0.00025350135,0.8216285,0.00009512894,0.00020936961,0.0015688067,0.0011192613,0.0012459396,0.13061349,0.0004909783,0.007404545,0.034627948],"study_design_scores_gemma":[0.000015986549,0.00009010526,0.9869212,0.0000048484876,0.00002602608,0.00020630888,0.00011361406,0.0005635276,0.005218773,0.000068480054,0.006761811,0.000009351741],"about_ca_topic_score_codex":0.00833946,"about_ca_topic_score_gemma":0.02220855,"teacher_disagreement_score":0.00833946,"about_ca_system_score_codex":0.00065929344,"about_ca_system_score_gemma":0.00027377336,"threshold_uncertainty_score":0.016581833},"labels":[],"label_agreement":null},{"id":"W4388289230","doi":"10.3847/1538-4357/acf863","title":"Astrochemical Modeling of Propargyl Radical Chemistry in TMC-1","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"National Science Foundation","keywords":"Propargyl; Physics; Astrochemistry; Molecular cloud; Radical; Astrophysics; Chemical physics; Polycyclic aromatic hydrocarbon; Interstellar medium; Chemistry; Photochemistry; Astrobiology; Organic chemistry; Stars; Galaxy","score_opus":0.013045235055620462,"score_gpt":0.24207186989172402,"score_spread":0.22902663483610355,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388289230","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99158174,0.00007435475,0.0034510454,0.00009160438,0.000016130967,0.00002885741,0.00070960936,0.00018586872,0.0038608434],"genre_scores_gemma":[0.9960188,0.000056739416,0.0026744956,0.00003386198,0.0000064521173,0.000024888926,0.00050023367,0.000058056652,0.000626421],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999212,0.000011191062,0.000002583996,0.000021262013,0.00001967497,0.000024082152],"domain_scores_gemma":[0.99978274,0.000070123395,0.000040189134,0.000024340286,0.000044837045,0.000037872556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022160436,0.0005286973,0.00038916993,0.00045156496,0.0006328669,0.0005972787,0.0009613206,0.00067880866,0.0021188993],"category_scores_gemma":[0.000629936,0.00026562178,0.0005804509,0.0004147089,0.00042084433,0.000570612,0.00045124354,0.0005092968,0.00027051038],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011886912,0.000082726496,0.019000191,0.000047493104,0.000046636906,0.000160112,0.000075654425,0.96515036,0.010804913,0.0023518945,0.00031172342,0.0018494584],"study_design_scores_gemma":[0.000041016974,0.00003454621,0.003295238,0.000002909814,0.000011683439,0.000019020787,0.00001871124,0.99302626,0.0024972353,0.0004966776,0.0005482084,0.0000085247975],"about_ca_topic_score_codex":0.031697083,"about_ca_topic_score_gemma":0.01416486,"teacher_disagreement_score":0.031697083,"about_ca_system_score_codex":0.0014200676,"about_ca_system_score_gemma":0.0009968067,"threshold_uncertainty_score":0.06302518},"labels":[],"label_agreement":null},{"id":"W4388413698","doi":"10.3847/1538-4357/acf2f4","title":"The Accretion History of EX Lup: A Century of Bursts, Outbursts, and Quiescence","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Key Research and Development Program of China; National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Accretion (finance)","score_opus":0.014204256186255964,"score_gpt":0.22466844180441886,"score_spread":0.2104641856181629,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388413698","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9915627,0.0008443905,0.0005224991,0.00016083663,0.000010664683,0.0000045981096,0.00088338665,0.000041519015,0.0059693977],"genre_scores_gemma":[0.9982796,0.00025521827,0.00024564218,0.000026802656,0.000025366806,0.0000032806977,0.00059443136,0.000016714946,0.00055302045],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998572,0.00002926877,0.0000134759075,0.000043815027,0.000031940654,0.000024308669],"domain_scores_gemma":[0.9988049,0.0003396752,0.0004487533,0.000097114935,0.00016199157,0.00014745675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007070478,0.00010961871,0.000120848716,0.0013786618,0.0004461514,0.0012333884,0.00021493016,0.00019151291,0.0014681701],"category_scores_gemma":[0.0025188434,0.000089947665,0.00010402728,0.0011307363,0.00035262748,0.0009781315,0.0008780186,0.00026809226,0.00025509665],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022073773,0.0000297059,0.9495045,0.00004836993,0.000047710662,0.00040693572,0.001349032,0.00074211764,0.0023270447,0.0013652893,0.0015941426,0.04236451],"study_design_scores_gemma":[0.0000025790362,0.000024072835,0.9909306,0.000027664757,0.000013359699,0.00018611443,0.00034440085,0.0014567096,0.00054875464,0.00061804644,0.005840371,0.0000073983665],"about_ca_topic_score_codex":0.005882106,"about_ca_topic_score_gemma":0.0059816707,"teacher_disagreement_score":0.005882106,"about_ca_system_score_codex":0.00055095914,"about_ca_system_score_gemma":0.00012764605,"threshold_uncertainty_score":0.011695743},"labels":[],"label_agreement":null},{"id":"W4388421290","doi":"10.3847/1538-4357/ad022e","title":"Erratum: “Changing-Look Quasar Candidates: First Results from Follow-up Spectroscopy of Highly Optically Variable Quasars” (2019, ApJ, 874, 8)","year":2023,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Quasar; Physics; Astrophysics; Spectroscopy; Astronomy; OVV quasar; Variable (mathematics); Galaxy","score_opus":0.008353665966875805,"score_gpt":0.2176013406814055,"score_spread":0.20924767471452968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388421290","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0018027683,0.0012847799,0.00038418768,0.10475695,0.8621251,0.00005265623,0.009894502,0.00058461184,0.019114427],"genre_scores_gemma":[0.02065606,0.0040711355,0.0037430269,0.20764239,0.17234722,0.00020620356,0.017014831,0.001798958,0.5725202],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9989868,0.00008741298,0.0001983568,0.00016039667,0.00043851614,0.00012855371],"domain_scores_gemma":[0.9906595,0.0020239498,0.00067196396,0.00059743656,0.0050504836,0.0009967142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014916401,0.0014802064,0.00091521034,0.003105961,0.0041491548,0.002463894,0.0017224754,0.003970161,0.07478042],"category_scores_gemma":[0.016235124,0.00068042206,0.00089141633,0.0014590459,0.00091253896,0.0015718035,0.0014269277,0.004126974,0.053797],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029432176,0.000010015628,0.00026854756,0.000020803034,0.0000029727569,0.00016008857,0.000010688875,0.000008881744,0.00004214429,0.00011190361,0.9968389,0.0024956646],"study_design_scores_gemma":[0.00009038635,0.00006513103,0.010504503,0.00032770203,0.00005224719,0.0009738275,0.0002844587,0.00017634638,0.0006036771,0.0010919231,0.9857604,0.000069406386],"about_ca_topic_score_codex":0.032132406,"about_ca_topic_score_gemma":0.057595465,"teacher_disagreement_score":0.07478042,"about_ca_system_score_codex":0.0020901333,"about_ca_system_score_gemma":0.003847528,"threshold_uncertainty_score":0.2501654},"labels":[],"label_agreement":null},{"id":"W4388421399","doi":"10.3847/1538-4357/ad0157","title":"Erratum: “Simple Physics and Integrators Accurately Reproduce Mercury Instability Statistics” (2023, ApJ, 944, 190)","year":2023,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Laser-induced spectroscopy and plasma","field":"Engineering","cited_by":0,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Integrator; Mercury (programming language); Instability; Statistical physics; Astrophysics; Mechanics; Quantum mechanics; Computer science","score_opus":0.02281405133553805,"score_gpt":0.264577300470597,"score_spread":0.24176324913505898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388421399","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0031335452,0.0014816923,0.0064573428,0.08309881,0.8259498,0.000075180265,0.008381233,0.0038327859,0.06758962],"genre_scores_gemma":[0.05706284,0.002386055,0.016554018,0.07549742,0.07381622,0.00018525789,0.009337654,0.007769771,0.7573907],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9985031,0.00016114181,0.00017563438,0.00023185153,0.0008149376,0.0001133624],"domain_scores_gemma":[0.9926972,0.001738149,0.0003389905,0.00070811727,0.0041913125,0.0003261537],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016055186,0.0013201974,0.000922744,0.002015821,0.0040047397,0.0035584301,0.0021374943,0.0035814461,0.07212341],"category_scores_gemma":[0.021620547,0.0007007252,0.0008688138,0.0013475188,0.0015448873,0.003629699,0.0014245041,0.0052855164,0.047230933],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004792674,0.000008661349,0.00012264027,0.000030088131,0.000005522411,0.000114052935,0.000021592201,0.0001562649,0.00017913262,0.0031202442,0.9912108,0.0049831364],"study_design_scores_gemma":[0.00008753502,0.000049875714,0.00290163,0.00016931233,0.00004742478,0.0005021134,0.00018925477,0.0044232933,0.002910049,0.02023153,0.9683648,0.00012324985],"about_ca_topic_score_codex":0.031389613,"about_ca_topic_score_gemma":0.03834471,"teacher_disagreement_score":0.07212341,"about_ca_system_score_codex":0.0031434468,"about_ca_system_score_gemma":0.0032973331,"threshold_uncertainty_score":0.24127686},"labels":[],"label_agreement":null},{"id":"W4388538935","doi":"10.3847/1538-4357/acf931","title":"Hidden Giants in JWST's PEARLS: An Ultramassive z = 4.26 Submillimeter Galaxy that Is Invisible to HST","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":55,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; National Astronomical Observatory of Japan; Max-Planck-Gesellschaft; Nuclear Safety and Security Commission; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; Academia Sinica; National Natural Science Foundation of China; United States-Israel Binational Science Foundation; Smithsonian Institution; Chinese Academy of Sciences South America Center for Astronomy; National Astronomical Research Institute of Thailand; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Galaxy; Astronomy; Astrophysics","score_opus":0.017686820700632152,"score_gpt":0.24449085320021,"score_spread":0.22680403249957784,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388538935","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988482,0.00002671765,0.00006602756,0.000030759158,0.0000013298154,0.0000019559532,0.000078585064,0.000022551274,0.00092386134],"genre_scores_gemma":[0.99901867,0.000026127347,0.00015990234,0.000040367457,0.0000055430064,0.0000011083073,0.00027598467,0.0000074670156,0.00046484312],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992955,0.0000032604542,0.0000026018665,0.000016607102,0.00002883267,0.000019136363],"domain_scores_gemma":[0.9997987,0.000015788546,0.000060892646,0.000016468482,0.000018831344,0.00008935126],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000093235416,0.00016638776,0.00019373339,0.0008800397,0.00039895365,0.0007520951,0.00022136446,0.00014289614,0.0017053734],"category_scores_gemma":[0.00023277759,0.00013770793,0.00009492766,0.0006294178,0.0004132369,0.00053387193,0.00080887205,0.00024080904,0.00030517604],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019028732,0.00009036031,0.9161522,0.00002684852,0.000051931045,0.0030993067,0.0030409205,0.00011786622,0.055222027,0.00077108014,0.0016906123,0.019546593],"study_design_scores_gemma":[0.000006225194,0.00004607338,0.9943855,0.000004368616,0.000012088391,0.0008655104,0.0007996899,0.00024888085,0.0012833918,0.00015982332,0.0021842613,0.0000042406896],"about_ca_topic_score_codex":0.004033809,"about_ca_topic_score_gemma":0.00855914,"teacher_disagreement_score":0.004033809,"about_ca_system_score_codex":0.00019443326,"about_ca_system_score_gemma":0.00008763803,"threshold_uncertainty_score":0.008020639},"labels":[],"label_agreement":null},{"id":"W4388653898","doi":"10.3847/1538-4357/acf843","title":"An X-Ray Census of Fast Radio Burst Host Galaxies: Constraints on Active Galactic Nuclei and X-Ray Counterparts","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"McGill Space Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Curtin University of Technology; McGill University; National Aeronautics and Space Administration; Fonds de recherche du Québec – Nature et technologies; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Population; Astronomy; Context (archaeology); Host (biology); Biology; Genetics","score_opus":0.014323638705669267,"score_gpt":0.2482688563811304,"score_spread":0.23394521767546111,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388653898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99818355,0.00012626997,0.00013891788,0.000013552635,0.0000012565177,0.000006990911,0.0010969285,0.000011042114,0.0004213324],"genre_scores_gemma":[0.9953733,0.00014748266,0.0003777875,0.000012405488,0.000008692274,0.000008288351,0.003799185,0.000008443961,0.00026443583],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970055,0.000034026132,0.00002658833,0.00007481728,0.00007618488,0.000087887005],"domain_scores_gemma":[0.99845636,0.00021690018,0.0004254868,0.0001595968,0.00025407752,0.00048751422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004699487,0.00023927151,0.00027915929,0.003118023,0.00027982253,0.0006551114,0.00029233922,0.0001841654,0.001516309],"category_scores_gemma":[0.001067939,0.00014433582,0.00017055993,0.0009725708,0.00019243326,0.00047559763,0.00093265506,0.00014841615,0.00065028825],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000703199,0.000023125307,0.98826724,0.0000140632155,0.000022806724,0.000093326984,0.00012107069,0.00009684815,0.005279954,0.00007754711,0.00023744174,0.005696279],"study_design_scores_gemma":[0.0000023624439,0.000027635087,0.9987453,0.000003580756,0.0000050778876,0.00017316215,0.0000716169,0.00020680373,0.00028678167,0.000018531924,0.00045722417,0.0000018366177],"about_ca_topic_score_codex":0.0059524993,"about_ca_topic_score_gemma":0.008404131,"teacher_disagreement_score":0.0059524993,"about_ca_system_score_codex":0.00017818039,"about_ca_system_score_gemma":0.00018306906,"threshold_uncertainty_score":0.011835694},"labels":[],"label_agreement":null},{"id":"W4388701351","doi":"10.3847/1538-4357/ad0043","title":"CWISE J105512.11+544328.3: A Nearby Y Dwarf Spectroscopically Confirmed with Keck/NIRES","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Rio Tinto (Canada); Espace pour la vie","funders":"Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Brown dwarf; Astrophysics; Metallicity; Stellar classification; Spectroscopy; Effective temperature; Astronomy; Luminosity; Stars; Galaxy","score_opus":0.010712750380578716,"score_gpt":0.23145868197079117,"score_spread":0.22074593159021244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388701351","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99551207,0.00015224308,0.00025972218,0.00011412131,0.000029263612,0.000016899918,0.00039425955,0.00004850858,0.0034727615],"genre_scores_gemma":[0.99644935,0.00005266726,0.00065048755,0.00018376842,0.000028253518,0.000012213962,0.0013047304,0.000029366654,0.0012892238],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997582,0.000007798336,0.000011046388,0.000082435494,0.000080396036,0.000060040737],"domain_scores_gemma":[0.99950886,0.00002632344,0.0001243031,0.000043562646,0.00008496435,0.0002120228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027608525,0.00050364033,0.00049287226,0.0009814921,0.001636998,0.0006442985,0.0005352331,0.0007359452,0.0017532486],"category_scores_gemma":[0.0003570959,0.00022958944,0.00027800974,0.00070685544,0.00055618084,0.00032273112,0.0010661945,0.0007199936,0.001038975],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00056647696,0.00034444706,0.79525393,0.00015129957,0.00015152614,0.009964515,0.0015659925,0.00044534434,0.17074588,0.00083007023,0.0052843853,0.014696161],"study_design_scores_gemma":[0.00003261144,0.00020431272,0.9817525,0.000024161494,0.00004055402,0.0035562343,0.0006996776,0.0005022482,0.0054868837,0.00017196932,0.007506814,0.000022069034],"about_ca_topic_score_codex":0.009218603,"about_ca_topic_score_gemma":0.017683676,"teacher_disagreement_score":0.009218603,"about_ca_system_score_codex":0.0005605179,"about_ca_system_score_gemma":0.00034260112,"threshold_uncertainty_score":0.018329918},"labels":[],"label_agreement":null},{"id":"W4388732176","doi":"10.3847/1538-4357/acffb9","title":"Magellanic System Stars Identified in SMACS J0723.3-7327 James Webb Space Telescope Early Release Observations Images","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Goddard Space Flight Center; Space Telescope Science Institute; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; European Space Agency; Arizona Space Grant Consortium","keywords":"Physics; Stars; Astrophysics; Astronomy; Large Magellanic Cloud; Galaxy; Star count; Distance modulus; Stellar density; Population; Photometry (optics); K-type main-sequence star; T Tauri star","score_opus":0.017664965529764785,"score_gpt":0.2291617567203541,"score_spread":0.2114967911905893,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388732176","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961901,0.000090343776,0.00006725969,0.000026853184,0.0000059846393,0.000007500566,0.001986252,0.000047274698,0.0015784374],"genre_scores_gemma":[0.991012,0.00008107439,0.00029644245,0.000037841095,0.000013126601,0.0000118706175,0.007734262,0.000015696123,0.0007977346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998287,0.000007682897,0.000009059921,0.000032640655,0.00006391632,0.000058060767],"domain_scores_gemma":[0.9993129,0.000026470412,0.00023390724,0.00004542562,0.00014497046,0.00023626146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016089968,0.0002201443,0.000239191,0.0024958134,0.0005226434,0.00054500205,0.00025735193,0.0001882982,0.0020473688],"category_scores_gemma":[0.00037017057,0.00011275716,0.00020626724,0.0013130502,0.00017653294,0.00016360926,0.0005106771,0.00016800496,0.00074668264],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000088378765,0.000044354656,0.9752171,0.000025075778,0.00006178058,0.00019439148,0.00018157213,0.00021155945,0.0134711685,0.00012552187,0.0042046886,0.006174283],"study_design_scores_gemma":[0.0000029489038,0.000009534269,0.9975915,0.0000039976553,0.000009269828,0.000065266715,0.0001029868,0.00017018852,0.0007020679,0.00001074919,0.0013285447,0.0000029864627],"about_ca_topic_score_codex":0.042710003,"about_ca_topic_score_gemma":0.10184337,"teacher_disagreement_score":0.042710003,"about_ca_system_score_codex":0.00070549664,"about_ca_system_score_gemma":0.00047960618,"threshold_uncertainty_score":0.08492279},"labels":[],"label_agreement":null},{"id":"W4388734078","doi":"10.3847/1538-4357/acf9f6","title":"Shadow Implications: What Does Measuring the Photon Ring Imply for Gravity?","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":29,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Shadow (psychology); Horizon; Observer (physics); Event horizon; Photon; Angular diameter; Nonparametric statistics; Metric (unit); Astrophysics; Astronomy; Theoretical physics; Optics; Quantum mechanics; Stars; Statistics","score_opus":0.027869127015174206,"score_gpt":0.2653525930680987,"score_spread":0.2374834660529245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388734078","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89609617,0.0005672058,0.086020015,0.0013501405,0.000057889745,0.000015504509,0.00035347108,0.00010607359,0.015433623],"genre_scores_gemma":[0.99765956,0.00008710822,0.001982764,0.00002619832,0.000027741093,0.0000035572757,0.000046993246,0.000009893269,0.00015610445],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9994167,0.00025284456,0.00002627191,0.00013587398,0.00011208475,0.00005613596],"domain_scores_gemma":[0.9886798,0.005178496,0.0026365332,0.0023251905,0.0006483703,0.000531672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016830805,0.00028309386,0.00040434636,0.00063451176,0.00048068698,0.0013101196,0.000616829,0.00043320347,0.0018313323],"category_scores_gemma":[0.016247816,0.00012701687,0.00019998103,0.0005606266,0.004228894,0.0037269157,0.0016193652,0.0007087958,0.00015474211],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055479555,0.00007187515,0.18262322,0.0002705746,0.00010293096,0.00067968684,0.0014790951,0.042761393,0.030024627,0.6632048,0.0022170974,0.07600997],"study_design_scores_gemma":[0.000029485265,0.00028784815,0.27737984,0.00011442147,0.00003557297,0.00091352727,0.0017590043,0.12124022,0.012217729,0.5808185,0.005067486,0.00013639948],"about_ca_topic_score_codex":0.0012008162,"about_ca_topic_score_gemma":0.000752133,"teacher_disagreement_score":0.0018313323,"about_ca_system_score_codex":0.00053223234,"about_ca_system_score_gemma":0.00025125768,"threshold_uncertainty_score":0.008901119},"labels":[],"label_agreement":null},{"id":"W4388767350","doi":"10.3847/1538-4357/acfb72","title":"Supermassive Black Holes with High Accretion Rates in Active Galactic Nuclei. XIII. Ultraviolet Time Lag of Hβ Emission in Mrk 142","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Western University","funders":"National Key Research and Development Program of China; Nuclear Safety and Security Commission; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Light curve; Active galactic nucleus; Observatory; Supermassive black hole; Emission spectrum; Accretion (finance); Ultraviolet; Astronomy; Telescope; Galaxy; Spectral line; Optics","score_opus":0.009144140345149933,"score_gpt":0.23329606115639442,"score_spread":0.2241519208112445,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388767350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992545,0.00009432659,0.0002603318,0.000008212726,0.0000020496386,0.0000033508177,0.00007443809,0.0000065697864,0.0002962684],"genre_scores_gemma":[0.9996598,0.000015734044,0.00014180184,0.000004271036,0.0000034972265,0.0000022899483,0.00007717031,0.0000016822978,0.000093868584],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999176,0.00001059765,0.000006962448,0.000031401356,0.000014211618,0.000019301347],"domain_scores_gemma":[0.9996542,0.00004197427,0.00021075385,0.00002471784,0.000023062512,0.000045239547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021316014,0.00018698178,0.00020331914,0.0004195889,0.00023707384,0.00041979091,0.00020306553,0.00016559781,0.00088922126],"category_scores_gemma":[0.0006179293,0.000105419116,0.00015994532,0.0002791601,0.00025823186,0.00027424254,0.0004422927,0.00019520006,0.00021151597],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034608797,0.00006645066,0.94321954,0.000025137204,0.00004002001,0.0007810456,0.00015459643,0.0005472052,0.048906464,0.00039274973,0.00011573285,0.0054049254],"study_design_scores_gemma":[0.00000604273,0.00006583245,0.99643904,0.0000023276168,0.000008659866,0.00029435597,0.00007613878,0.0006497709,0.002108027,0.00016645805,0.00018011578,0.000003231428],"about_ca_topic_score_codex":0.0013529074,"about_ca_topic_score_gemma":0.0017885613,"teacher_disagreement_score":0.0013529074,"about_ca_system_score_codex":0.00016832887,"about_ca_system_score_gemma":0.000102718026,"threshold_uncertainty_score":0.002974689},"labels":[],"label_agreement":null},{"id":"W4388824194","doi":"10.3847/1538-4357/acf833","title":"Gas-phase Metallicity of Local Active Galactic Nuclei in the GASP and MaNGA Surveys: The Role of Ram Pressure Stripping","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; Deutsche Forschungsgemeinschaft; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; HORIZON EUROPE European Research Council; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ministero dell’Istruzione, dell’Università e della Ricerca; Carnegie Mellon University; Universidad Nacional Autónoma de México; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik; European Commission","keywords":"Physics; Metallicity; Galaxy; Photoionization; Astrophysics; Stars; Active galactic nucleus; Ionization; Ion","score_opus":0.010554267518660454,"score_gpt":0.2379484265460191,"score_spread":0.22739415902735866,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388824194","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980141,0.00022728092,0.00020824233,0.00005874434,0.0000018411669,0.0000024443123,0.00048299498,0.000012115622,0.0009921828],"genre_scores_gemma":[0.9995635,0.000031436524,0.000057007957,0.0000055176893,0.000003176345,0.0000011195464,0.00023591405,0.0000024186515,0.000099897916],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975353,0.00008826983,0.000013648642,0.00007169685,0.000031279647,0.000041514944],"domain_scores_gemma":[0.99845266,0.0004303636,0.00058937154,0.00014145943,0.00012941986,0.00025666563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006811646,0.00015958733,0.00018486845,0.00086421287,0.00020800425,0.00059590413,0.0003629117,0.0001602155,0.0013756624],"category_scores_gemma":[0.0019946662,0.000103046885,0.00018051325,0.00072545494,0.00044129204,0.00057343923,0.00045727452,0.00018883435,0.0003865617],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000023759298,0.0000022429504,0.99808854,0.000006334976,0.000016772647,0.00001909268,0.0000615457,0.000066251305,0.0004338292,0.000049807586,0.000052439445,0.0011793846],"study_design_scores_gemma":[4.947994e-7,0.000005405273,0.99943,0.0000023946259,0.0000048526404,0.000021200414,0.000107038344,0.00020726983,0.00010572907,0.000022194907,0.000092704926,8.391566e-7],"about_ca_topic_score_codex":0.009954204,"about_ca_topic_score_gemma":0.011960974,"teacher_disagreement_score":0.009954204,"about_ca_system_score_codex":0.00024388051,"about_ca_system_score_gemma":0.00013573651,"threshold_uncertainty_score":0.019792557},"labels":[],"label_agreement":null},{"id":"W4388834284","doi":"10.3847/1538-4357/acff6d","title":"Mass and Angular Momentum Transport in a Gravitationally Unstable Protoplanetary Disk with Improved 3D Radiative Hydrodynamics","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Protoplanetary disk; Radiative transfer; Angular momentum; Astrophysics; Planet; Accretion (finance); Radiative cooling; Mechanics; Mass distribution; Gravitation; Classical mechanics; Galaxy; Optics","score_opus":0.004172220954218297,"score_gpt":0.2017081205859834,"score_spread":0.1975358996317651,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388834284","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913564,0.000074475865,0.005674797,0.00012824014,0.000014000342,0.000016494892,0.00019016628,0.0003465969,0.0021987853],"genre_scores_gemma":[0.9958099,0.00003109722,0.0037922647,0.000018668075,0.000009776825,0.000010958749,0.00008647126,0.000041470055,0.00019940948],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999137,0.000022992635,0.0000057585567,0.000016573094,0.00002130539,0.00001965886],"domain_scores_gemma":[0.9996537,0.00011680291,0.00007273327,0.00006781485,0.00005316948,0.00003585348],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021050076,0.0004111575,0.00038515654,0.00047457303,0.00039196014,0.0008033534,0.00081480364,0.00046442595,0.0011100121],"category_scores_gemma":[0.0008946586,0.0002711683,0.00055263063,0.0003756407,0.0006832305,0.00035771567,0.00047788298,0.00042756012,0.00012845267],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016731444,0.00012474992,0.011774102,0.000031051408,0.000055752153,0.00028151515,0.00013376006,0.9642522,0.01773526,0.0014477808,0.00027263275,0.0037238975],"study_design_scores_gemma":[0.000032557648,0.000021914613,0.0037063495,0.0000018993635,0.0000059049803,0.000016793065,0.000016790085,0.99517703,0.000691243,0.00020995607,0.00011164558,0.000007994712],"about_ca_topic_score_codex":0.014293787,"about_ca_topic_score_gemma":0.00526607,"teacher_disagreement_score":0.014293787,"about_ca_system_score_codex":0.0011737272,"about_ca_system_score_gemma":0.00059984653,"threshold_uncertainty_score":0.028421164},"labels":[],"label_agreement":null},{"id":"W4388866047","doi":"10.3847/1538-4357/ad0294","title":"Variability as a Predictor for the Hard-to-soft State Transition in GX 339−4","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Astrophysics Science Division; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Goddard Space Flight Center; Nuclear Safety and Security Commission; Deutsches Zentrum für Luft- und Raumfahrt; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Black-body radiation; Accretion (finance); Black hole (networking); Luminosity; Corona (planetary geology); Astronomy; Accretion disc; Galaxy; Radiation","score_opus":0.016667879449903573,"score_gpt":0.25031502979742454,"score_spread":0.23364715034752095,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388866047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99952435,0.000026709738,0.000117857446,0.000007919259,0.0000015580878,0.000001781885,0.00018435996,0.000006855136,0.00012863957],"genre_scores_gemma":[0.9995414,0.000010743713,0.00006307028,0.0000025533868,0.0000037783964,0.0000017427453,0.00031982543,0.000002649535,0.00005439306],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991333,0.0000142182125,0.000008003795,0.000029044955,0.000015477443,0.000019932115],"domain_scores_gemma":[0.9990256,0.00027042665,0.00037947865,0.000090580186,0.000067496694,0.0001664843],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002737757,0.00016792072,0.00018753402,0.0009016426,0.0002273772,0.0005366387,0.00015825972,0.00026605188,0.0014797928],"category_scores_gemma":[0.001136077,0.00011293007,0.00019330789,0.0004932821,0.00019633105,0.00028058523,0.00046953114,0.0003477996,0.0001988994],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001159993,0.000026664753,0.9915941,0.000006298408,0.000023039278,0.00005882108,0.0000882641,0.00031246836,0.005959936,0.000046181434,0.00006701683,0.001701169],"study_design_scores_gemma":[6.9962897e-7,0.00001252588,0.999276,9.298059e-7,0.0000024170242,0.000026393564,0.000026402979,0.00041661534,0.00018236325,0.000013892417,0.000040593106,0.0000010781],"about_ca_topic_score_codex":0.0018180497,"about_ca_topic_score_gemma":0.0019388213,"teacher_disagreement_score":0.0018180497,"about_ca_system_score_codex":0.00015578022,"about_ca_system_score_gemma":0.000058812213,"threshold_uncertainty_score":0.004950464},"labels":[],"label_agreement":null},{"id":"W4388907476","doi":"10.3847/1538-4357/ad0030","title":"Metallicity Distribution Functions of 13 Ultra-faint Dwarf Galaxy Candidates from Hubble Space Telescope Narrowband Imaging","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Metallicity; Galaxy; Stars; Dwarf galaxy; Astronomy; Reionization; Luminosity; Stellar mass; Milky Way; Luminosity function; Hubble space telescope; Star formation; Redshift","score_opus":0.008785463426493185,"score_gpt":0.21993936024972374,"score_spread":0.21115389682323055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388907476","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991339,0.000050793475,0.00017432563,0.0000043801556,6.1454125e-7,0.0000017902131,0.00041463543,0.000017641494,0.0002019582],"genre_scores_gemma":[0.99800366,0.00002236744,0.0002675272,0.000005462298,0.0000021173862,0.0000032192631,0.0015080229,0.0000065047657,0.0001810834],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997911,0.000019765346,0.000016607464,0.000061697094,0.000050193885,0.00006069164],"domain_scores_gemma":[0.9988662,0.00017138924,0.0003448213,0.00014235223,0.00019843294,0.00027681497],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039282307,0.00027141665,0.00033769436,0.0024274255,0.00031738772,0.0005702176,0.00029074098,0.0002168422,0.0011936721],"category_scores_gemma":[0.00090366893,0.00013996614,0.00027175585,0.0010864752,0.00022874406,0.00026294636,0.0004886718,0.000115351584,0.0004732727],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006598726,0.000012564307,0.9877413,0.000008933957,0.00002406546,0.00005755967,0.00012518172,0.00020311384,0.005328555,0.000040289917,0.00016357913,0.006228913],"study_design_scores_gemma":[0.0000010568568,0.0000122165075,0.9984285,0.0000015867118,0.0000054998354,0.000092376074,0.00004479929,0.00037814348,0.00079206657,0.000016492846,0.00022499371,0.0000022694549],"about_ca_topic_score_codex":0.0046684737,"about_ca_topic_score_gemma":0.0070566214,"teacher_disagreement_score":0.0046684737,"about_ca_system_score_codex":0.00038467365,"about_ca_system_score_gemma":0.000096258336,"threshold_uncertainty_score":0.009282589},"labels":[],"label_agreement":null},{"id":"W4388926090","doi":"10.3847/1538-4357/ad1a10","title":"Chasing the Break: Tracing the Full Evolution of a Black Hole X-Ray Binary Jet with Multiwavelength Spectral Modeling","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Lethbridge; McGill University","funders":"Science and Technology Facilities Council; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; European Southern Observatory; Max-Planck-Gesellschaft; Tamkeen; Academia Sinica; National Radio Astronomy Observatory; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Space Telescope Science Institute; New York University Abu Dhabi; McGill University; Canada Research Chairs; Nuclear Safety and Security Commission; Ministerio de Ciencia, Innovación y Universidades; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Astronomical Research Institute of Thailand; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; National Science Foundation","keywords":"Astrophysics; Physics; Accretion (finance); Black hole (networking); Jet (fluid); Astronomy; Spectral line; Inflow; Outflow; Radio spectrum; Radiative transfer; Mechanics; Meteorology","score_opus":0.013528800142701705,"score_gpt":0.22852050365827525,"score_spread":0.21499170351557356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388926090","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889681,0.00017048814,0.0091938265,0.00010493948,0.000008842704,0.000009649585,0.00042435774,0.00016032506,0.00095950684],"genre_scores_gemma":[0.9920887,0.00008219386,0.0070365644,0.00001807172,0.000012806801,0.000010244279,0.00050852704,0.000038085134,0.00020487599],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999229,0.000014833523,0.000004435664,0.00002891004,0.000014885958,0.000014103005],"domain_scores_gemma":[0.9997304,0.00007536974,0.000088400135,0.000040251853,0.000026364125,0.000039186605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003502554,0.00027635437,0.00018676119,0.000879667,0.00026198593,0.00075387204,0.0005442299,0.00033318155,0.00052508037],"category_scores_gemma":[0.0008459895,0.00023350268,0.00040856822,0.00036883308,0.00020616147,0.0005044386,0.00046447065,0.00032528883,0.00016144171],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025746465,0.00031386546,0.61515707,0.000075901415,0.00023617545,0.0003652616,0.00048667003,0.32727695,0.025171813,0.003516466,0.0009607864,0.026181515],"study_design_scores_gemma":[0.000009991776,0.000035719124,0.16492802,0.000012739447,0.000026653424,0.00006741069,0.00013256376,0.8309589,0.0016201311,0.001438793,0.00075485924,0.000014160603],"about_ca_topic_score_codex":0.008369841,"about_ca_topic_score_gemma":0.007679318,"teacher_disagreement_score":0.008369841,"about_ca_system_score_codex":0.00043267253,"about_ca_system_score_gemma":0.00023396824,"threshold_uncertainty_score":0.016642213},"labels":[],"label_agreement":null},{"id":"W4388969986","doi":"10.3847/1538-4357/acf9ee","title":"The Stability of Some Galaxy Disks is Still Perplexing","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Galaxy; Astrophysics; Instability; Bulge; RADIUS; Bar (unit); Galaxy formation and evolution; Astronomy; Mechanics","score_opus":0.015170375124143725,"score_gpt":0.2395513571568386,"score_spread":0.22438098203269485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388969986","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9882968,0.0003914825,0.0066028093,0.00077128806,0.00002414393,0.0000057600087,0.00005504645,0.00010019586,0.0037523408],"genre_scores_gemma":[0.9987557,0.00006742661,0.0006439604,0.00003650797,0.000005290596,0.0000019802912,0.000015990225,0.000012789641,0.00046035164],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993217,0.000019454608,0.0000034436823,0.000016549755,0.000011640432,0.000016710188],"domain_scores_gemma":[0.99959,0.0001553672,0.00007468198,0.0000641196,0.000046744768,0.000069084024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022259541,0.00021943453,0.0002971933,0.00026647202,0.00077393523,0.00123066,0.00048120963,0.00073944964,0.0021354598],"category_scores_gemma":[0.0014428962,0.0001790592,0.00027929453,0.00013854244,0.001098212,0.001063052,0.00050859456,0.00046612992,0.00021960886],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003881382,0.00015394083,0.109464645,0.00036953087,0.00043395234,0.0007783224,0.0017443955,0.6984427,0.09607401,0.062431384,0.0026690993,0.027049946],"study_design_scores_gemma":[0.00012041198,0.00035654602,0.0441195,0.0000669687,0.00016470977,0.0003726426,0.0012839537,0.8457408,0.02226729,0.076288715,0.009113148,0.00010525974],"about_ca_topic_score_codex":0.00573994,"about_ca_topic_score_gemma":0.0041087954,"teacher_disagreement_score":0.00573994,"about_ca_system_score_codex":0.00065147434,"about_ca_system_score_gemma":0.00024986683,"threshold_uncertainty_score":0.011413038},"labels":[],"label_agreement":null},{"id":"W4388970066","doi":"10.3847/1538-4357/acffc9","title":"SN 2022joj: A Peculiar Type Ia Supernova Possibly Driven by an Asymmetric Helium-shell Double Detonation","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"H2020 European Research Council; Deutsches Elektronen-Synchrotron; University of California Observatories; Stockholms Universitet; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Horizon 2020 Framework Programme; Aarhus Universitet; Turun Yliopisto; Nuclear Safety and Security Commission; Háskóli Íslands; Universitetet i Oslo; Queen's University; Irish Research Council; University of Warwick; Weizmann Institute of Science; W. M. Keck Foundation; Space Telescope Science Institute; Smithsonian Institution; Vetenskapsrådet; Northwestern University; California Institute of Technology; Gordon and Betty Moore Foundation; Queen's University Belfast; National Aeronautics and Space Administration; Trinity College Dublin; National Science Foundation","keywords":"Physics; Supernova; Shell (structure); Helium; Detonation; Astrophysics; Type (biology); Astronomy; Atomic physics; Explosive material","score_opus":0.015958136996534096,"score_gpt":0.2650325771777595,"score_spread":0.24907444018122543,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4388970066","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9908839,0.00023424876,0.0009798375,0.00010675555,0.00009743667,0.000033072873,0.0012519178,0.00022741657,0.0061853677],"genre_scores_gemma":[0.9952744,0.00006791376,0.00075760315,0.00013924397,0.000050674,0.000014745258,0.0020403431,0.00003922526,0.001615783],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99992967,0.0000029307048,0.0000032469504,0.000019609573,0.00001555547,0.000029047009],"domain_scores_gemma":[0.9998292,0.000009235876,0.000023652728,0.00002215599,0.000016875849,0.00009883267],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012737443,0.00065205793,0.0003517842,0.0005628309,0.0005784001,0.00059219834,0.00032991674,0.00068000326,0.002103503],"category_scores_gemma":[0.0002014107,0.00023317608,0.00035586956,0.00036908034,0.00021227523,0.00025416512,0.00075649086,0.0004818697,0.00069428823],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0035954695,0.00045045087,0.31920758,0.00027431114,0.00047995607,0.03806455,0.00025940142,0.002745997,0.59511065,0.0030177508,0.013618775,0.023175215],"study_design_scores_gemma":[0.00019224676,0.0008201781,0.923632,0.000027974525,0.00012362482,0.014856784,0.00022489474,0.0078261485,0.029183319,0.0009148133,0.022111552,0.000086535714],"about_ca_topic_score_codex":0.0032964996,"about_ca_topic_score_gemma":0.006230125,"teacher_disagreement_score":0.0032964996,"about_ca_system_score_codex":0.0002807509,"about_ca_system_score_gemma":0.00014137158,"threshold_uncertainty_score":0.0070369244},"labels":[],"label_agreement":null},{"id":"W4389049117","doi":"10.3847/1538-4357/acfdac","title":"AGN STORM 2. IV. Swift X-Ray and Ultraviolet/Optical Monitoring of Mrk 817","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council; Youth Innovation Promotion Association of the Chinese Academy of Sciences; University of California, Irvine; Chinese Academy of Sciences; National Natural Science Foundation of China; University of Leicester; Alexander von Humboldt-Stiftung; National Aeronautics and Space Administration; Nuclear Safety and Security Commission; Youth Innovation Promotion Association; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Light curve; Astrophysics; Ultraviolet; Flare; Emission spectrum; Wavelength; Amplitude; Active galactic nucleus; Torus; Galaxy; Accretion disc; Quasar; Astronomy; Spectral line; Optics; Geometry","score_opus":0.01684867147506799,"score_gpt":0.24843425360668414,"score_spread":0.23158558213161615,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389049117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99346924,0.000037385496,0.00035292786,0.000044997396,0.000013344455,0.00003338611,0.0025585692,0.0001337888,0.0033563206],"genre_scores_gemma":[0.989298,0.000029077813,0.001312073,0.000070449256,0.00003300798,0.000034444784,0.007949752,0.0000479751,0.0012252243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998349,0.000010366019,0.000007747709,0.000042692616,0.00005707512,0.000047204798],"domain_scores_gemma":[0.99959177,0.000025158923,0.00010841548,0.00004469248,0.000098148026,0.00013174227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003130647,0.0003110073,0.00030461446,0.00058480457,0.00051827775,0.00054208783,0.0002835604,0.00038390266,0.00080345705],"category_scores_gemma":[0.00030247236,0.0001656951,0.0002395571,0.00029269423,0.00014133991,0.00025088282,0.00040460355,0.00044430434,0.00072414504],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012577327,0.0004955874,0.86121273,0.000083633975,0.00018636124,0.0023843024,0.00072418526,0.0028038195,0.10147719,0.00033173457,0.007603619,0.021439016],"study_design_scores_gemma":[0.000026591544,0.00021106972,0.99008614,0.0000067521114,0.000022033732,0.000330238,0.00009660978,0.0022113842,0.004357118,0.000046097488,0.0025950186,0.000010855404],"about_ca_topic_score_codex":0.0058671017,"about_ca_topic_score_gemma":0.013836211,"teacher_disagreement_score":0.0058671017,"about_ca_system_score_codex":0.00036748304,"about_ca_system_score_gemma":0.00026517946,"threshold_uncertainty_score":0.011665881},"labels":[],"label_agreement":null},{"id":"W4389051159","doi":"10.3847/1538-4357/acfdfb","title":"PEARLS: JWST Counterparts of Microjansky Radio Sources in the Time Domain Field","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Astrophysics Division; Science and Technology Facilities Council; University of Arizona; National Astronomical Observatory of Japan; U.S. Naval Research Laboratory; National Research Foundation of Korea; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; European Research Council; Nuclear Safety and Security Commission; Space Telescope Science Institute; Goddard Space Flight Center; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Redshift; Galaxy; Astronomy; Star formation","score_opus":0.005491089210188872,"score_gpt":0.20703939935236068,"score_spread":0.2015483101421718,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389051159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98993206,0.00013624928,0.00036083366,0.0001243468,0.000020428904,0.000011468586,0.0006439442,0.0000665201,0.008704255],"genre_scores_gemma":[0.9960801,0.000048128568,0.0003140835,0.000066703826,0.000038504983,0.00000522391,0.0014430118,0.000033215787,0.0019709908],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998233,0.0000085031,0.0000109970515,0.000044174696,0.00006816894,0.000044962526],"domain_scores_gemma":[0.99898595,0.00009014022,0.00036015705,0.00013703854,0.00013221265,0.0002945631],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024248102,0.00020680841,0.00013960159,0.0017021091,0.0005149483,0.0009551006,0.0002928402,0.00017726648,0.007040272],"category_scores_gemma":[0.0011785164,0.00014403362,0.000088463305,0.0010151056,0.0003991189,0.0006702528,0.0013805052,0.00037128705,0.0014143075],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032471196,0.00012829884,0.9213512,0.00004171073,0.000051968484,0.0055982196,0.0016116592,0.00014420804,0.021403128,0.0023649642,0.006929161,0.0400507],"study_design_scores_gemma":[0.000022937686,0.00005863088,0.9824091,0.000020973142,0.000011703195,0.003603276,0.000504106,0.0002483529,0.0016668793,0.0005761556,0.010871005,0.0000069443563],"about_ca_topic_score_codex":0.0027968518,"about_ca_topic_score_gemma":0.0047357036,"teacher_disagreement_score":0.007040272,"about_ca_system_score_codex":0.00015708881,"about_ca_system_score_gemma":0.00009769836,"threshold_uncertainty_score":0.023552},"labels":[],"label_agreement":null},{"id":"W4389057323","doi":"10.3847/1538-4357/ad04db","title":"Σ<sub>SFR</sub>–M <sub>∗</sub> Diagram: A Valuable Galaxy Evolution Diagnostic to Complement (s)SFR–M <sub>∗</sub> Diagrams","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Nuclear Safety and Security Commission; National Aeronautics and Space Administration","keywords":"Physics; Galaxy; Astrophysics; Star formation; Redshift; Effective radius; Diagram; Stellar mass; Galaxy formation and evolution; RADIUS; Astronomy; Statistics","score_opus":0.011744314056872469,"score_gpt":0.22759297111235044,"score_spread":0.21584865705547798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389057323","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9134703,0.0006684897,0.022410866,0.0004133351,0.00007572962,0.000042455194,0.006910758,0.002204354,0.053803742],"genre_scores_gemma":[0.9944792,0.000026279195,0.0037899339,0.000032897806,0.000023261835,0.00000917517,0.0009263921,0.00007846155,0.00063449354],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998136,0.000039559207,0.000016919803,0.000034442513,0.00005670698,0.000038716964],"domain_scores_gemma":[0.9974981,0.0009736454,0.0005569606,0.00019099328,0.0004619603,0.00031824945],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047271792,0.00020957235,0.00021694125,0.0028328719,0.00019899424,0.00095112406,0.00020882735,0.00031550578,0.0076118424],"category_scores_gemma":[0.002452854,0.000053404478,0.00018333652,0.00086434337,0.00029720264,0.0006672556,0.000567253,0.00022036166,0.0016530764],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006007666,0.000062502324,0.82477045,0.00015827504,0.00009685369,0.00053853734,0.0007645696,0.0026672592,0.027124383,0.026947942,0.0118223475,0.10444622],"study_design_scores_gemma":[0.000015678186,0.00011067573,0.92004025,0.000050732644,0.000030172117,0.0015711716,0.0005119527,0.016278166,0.009959183,0.014050787,0.037349127,0.000032121297],"about_ca_topic_score_codex":0.0013289631,"about_ca_topic_score_gemma":0.0010106378,"teacher_disagreement_score":0.0076118424,"about_ca_system_score_codex":0.00025991173,"about_ca_system_score_gemma":0.00013999043,"threshold_uncertainty_score":0.025464118},"labels":[],"label_agreement":null},{"id":"W4389078871","doi":"10.3847/1538-4357/ad05c0","title":"Bridging the Gap between Cosmic Dawn and Reionization Favors Models Dominated by Faint Galaxies","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"University Grants Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Reionization; Physics; Astrophysics; Redshift; Galaxy; Dark Ages; Optical depth; Star formation; COSMIC cancer database; Halo; Astronomy; Galaxy formation and evolution","score_opus":0.012627579878477771,"score_gpt":0.21989230744131227,"score_spread":0.2072647275628345,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389078871","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9845989,0.000097975884,0.013322179,0.00029368486,0.000007532564,0.000009941116,0.00010048228,0.000086759035,0.0014825363],"genre_scores_gemma":[0.9991074,0.000023973038,0.00059191417,0.00002837937,0.000006627996,0.00000387116,0.00005078336,0.000018852721,0.0001682276],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995696,0.00016578841,0.000016090882,0.00013789455,0.000032784574,0.00007783979],"domain_scores_gemma":[0.994974,0.0031311375,0.0009081679,0.00038748383,0.00013380704,0.00046534435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002824655,0.00044491253,0.0008042779,0.0005830617,0.0003696291,0.0013603106,0.0016836422,0.0007734217,0.0019867367],"category_scores_gemma":[0.007453253,0.0004129538,0.0004967859,0.00027426452,0.0009794179,0.0014859905,0.001090418,0.0006529724,0.00018379527],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067456026,0.00019762953,0.1841575,0.00010659291,0.0002916323,0.00055370043,0.0005778504,0.739014,0.0041982117,0.05911907,0.0006857953,0.010423401],"study_design_scores_gemma":[0.0000377031,0.00006227719,0.016838804,0.000011292532,0.000029774395,0.000052935895,0.00009057296,0.9685458,0.00038364192,0.013690666,0.00024105846,0.00001543724],"about_ca_topic_score_codex":0.0076535516,"about_ca_topic_score_gemma":0.0056566917,"teacher_disagreement_score":0.0076535516,"about_ca_system_score_codex":0.0013268333,"about_ca_system_score_gemma":0.0005586748,"threshold_uncertainty_score":0.0152180195},"labels":[],"label_agreement":null},{"id":"W4389143237","doi":"10.3847/1538-4357/acf4f2","title":"A Search for Pulsars around Sgr A* in the First Event Horizon Telescope Data Set","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; University of Waterloo; Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; McGill University; Canadian Institute for Advanced Research","funders":"Los Alamos National Laboratory; Oak Ridge National Laboratory; High Energy Physics; Office of International Science and Engineering; National Key Research and Development Program of China; Japan Society for the Promotion of Science; Physics Division, National Center for Theoretical Sciences; Astrophysics Division; Jet Propulsion Laboratory; National Nuclear Security Administration; Toray Science Foundation; East Asian Core Observatories Association; Institut Périmètre de physique théorique; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Recruitment Program of Global Experts; Universidad Nacional Autónoma de México; Ministry of Education, India; European Research Council; Centre National de la Recherche Scientifique; Academy of Finland; Max-Planck-Gesellschaft; National Natural Science Foundation of China; National Research Foundation of Korea; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Generalitat Valenciana; National Science Foundation; China Postdoctoral Science Foundation; Instituto de Astrofísica de Andalucía; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Chinese Academy of Sciences; Academia Sinica; Junta de Andalucía; Universiteit van Amsterdam; Leverhulme Trust; European Commission; National Radio Astronomy Observatory; Fundação de Amparo à Pesquisa do Estado de São Paulo; Natural Sciences and Engineering Research Council of Canada; Bureau of International Cooperation, Chinese Academy of Sciences; European Southern Observatory; John Templeton Foundation; China Scholarship Council; Ministry of Education, Culture, Sports, Science and Technology; Radboud Universiteit; University of Pretoria; National Research Foundation; Office of Science; Simons Foundation; Joint Institute for Computational Fundamental Science; Precursory Research for Embryonic Science and Technology; University of Arizona; Smithsonian Institution; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Vetenskapsrådet; U.S. Department of Energy; Korea Astronomy and Space Science Institute; Science and Technology Facilities Council; Universiteit Leiden; Associated Universities; Space Telescope Science Institute; National Astronomical Observatory of Japan; Canadian Institute for Advanced Research; California Institute of Technology; National Institutes of Natural Sciences; Government of Canada; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Ministerio de Ciencia e Innovación; Consejo Nacional de Ciencia y Tecnología; Consejo Superior de Investigaciones Científicas; University of Chicago; National Center for Theoretical Sciences; National Aeronautics and Space Administration; Gordon and Betty Moore Foundation; Brinson Foundation; Flatiron Health","keywords":"Physics; Pulsar; Astronomy; Event (particle physics); Astrophysics; Telescope; Event horizon; Set (abstract data type); Data set; Horizon; Artificial intelligence","score_opus":0.054449996938466104,"score_gpt":0.383674491113412,"score_spread":0.3292244941749459,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389143237","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99181515,0.00012132331,0.0009465734,0.00006838868,0.000012945349,0.000023558323,0.0061814142,0.00012684733,0.000703797],"genre_scores_gemma":[0.95802647,0.00007311127,0.0032289464,0.000042452684,0.00003462152,0.000027311506,0.038026683,0.000047206075,0.0004932153],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993641,0.00008354363,0.000055527045,0.00015069135,0.00022279745,0.00012334471],"domain_scores_gemma":[0.9983278,0.0004677323,0.00035561362,0.00023226581,0.00023492055,0.00038164403],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081292767,0.00033157817,0.0005132214,0.0027642432,0.00050715,0.00081262796,0.00044072032,0.00035852107,0.0011808713],"category_scores_gemma":[0.0016807208,0.00016874379,0.00057760463,0.001801047,0.00019608017,0.00028424925,0.000945792,0.00032200242,0.00053554645],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052302633,0.00019820513,0.93243766,0.00010474153,0.0003119412,0.00074787426,0.00031150036,0.0020707368,0.02420668,0.00030276735,0.0041873762,0.034597617],"study_design_scores_gemma":[0.0000385099,0.000108886496,0.98443407,0.000014532786,0.00007440647,0.00031856625,0.0001744697,0.0065181823,0.0043652006,0.00011143719,0.0038272727,0.00001443627],"about_ca_topic_score_codex":0.006410624,"about_ca_topic_score_gemma":0.008752356,"teacher_disagreement_score":0.006410624,"about_ca_system_score_codex":0.00040727563,"about_ca_system_score_gemma":0.00052201253,"threshold_uncertainty_score":0.012746632},"labels":[],"label_agreement":null},{"id":"W4389162759","doi":"10.3847/1538-4357/ad09e4","title":"How to Detect an Astrophysical Nanohertz Gravitational Wave Background","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Office of Naval Research; Science and Technology Facilities Council; College of Science, Oregon State University; Goddard Space Flight Center; Jet Propulsion Laboratory; Deutsche Forschungsgemeinschaft; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; Flatiron Health; Associated Universities; Oregon State University; Canadian Institute for Advanced Research; Space Telescope Science Institute; California Institute of Technology; National Aeronautics and Space Administration; Vanderbilt University; Research Corporation for Science Advancement; National Science Foundation","keywords":"Physics; Gravitational wave background; Gravitational wave; Astrophysics; Superposition principle; Spectral density; Pulsar; Statistical physics; Data set; Cosmic variance; Set (abstract data type); Cosmology; Statistical hypothesis testing; Noise (video); Redshift; Statistics; Quantum mechanics","score_opus":0.03102664034863516,"score_gpt":0.32985132738817097,"score_spread":0.2988246870395358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389162759","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88676333,0.00017541023,0.109337255,0.00094601914,0.00005089014,0.000026242284,0.0004241452,0.00027985816,0.0019969237],"genre_scores_gemma":[0.970922,0.00007982998,0.028194657,0.00010524251,0.000020755044,0.000016463338,0.0004058743,0.000045713932,0.00020945228],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9994142,0.00019950524,0.00003240182,0.00017797937,0.0001358638,0.000040120758],"domain_scores_gemma":[0.99233586,0.005033812,0.0009269291,0.00091511535,0.0004942495,0.0002940202],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024791898,0.00021681965,0.0003793191,0.0006844068,0.0002855672,0.0015571186,0.0005784971,0.0005877897,0.0011183663],"category_scores_gemma":[0.014699973,0.00035935565,0.00029386076,0.0006416053,0.0006679689,0.0016246971,0.0005974669,0.00065224536,0.0003788533],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042693413,0.00035660903,0.4594508,0.0001792958,0.00042791324,0.00027710566,0.0003221399,0.28221366,0.050397776,0.036197685,0.0036037504,0.16614626],"study_design_scores_gemma":[0.00004913462,0.00014878705,0.11884164,0.00003592809,0.00005911125,0.00024558083,0.00022183778,0.8189258,0.021297177,0.037076775,0.0030366094,0.0000616809],"about_ca_topic_score_codex":0.002430684,"about_ca_topic_score_gemma":0.0018292998,"teacher_disagreement_score":0.0024791898,"about_ca_system_score_codex":0.0004252199,"about_ca_system_score_gemma":0.00061402784,"threshold_uncertainty_score":0.0131114125},"labels":[],"label_agreement":null},{"id":"W4389327075","doi":"10.3847/1538-4357/acf712","title":"JWST's TEMPLATES for Star Formation: The First Resolved Gas-phase Metallicity Maps of Dust-obscured Star-forming Galaxies at z ∼ 4","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; National Radio Astronomy Observatory; Goddard Space Flight Center; National Astronomical Observatory of Japan; Max-Planck-Gesellschaft; Space Telescope Science Institute; Alfred P. Sloan Foundation; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Oak Ridge Associated Universities; National Science Foundation","keywords":"Physics; Astrophysics; Metallicity; Galaxy; Star formation; Astronomy; Submillimeter Array; Interstellar medium; Millimeter; Luminous infrared galaxy; James Webb Space Telescope; Active galactic nucleus; Dust lane","score_opus":0.01940952964898358,"score_gpt":0.24607474516318206,"score_spread":0.2266652155141985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389327075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9933674,0.000049631682,0.0007727223,0.000020416703,0.000002073455,0.000011988816,0.0040584086,0.000093712035,0.0016236407],"genre_scores_gemma":[0.98961395,0.000026875961,0.0015324946,0.000010866039,0.000005512646,0.000007718098,0.008444113,0.000034766817,0.00032371192],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986136,0.000009729821,0.000009663738,0.000036276102,0.00005066924,0.000032315656],"domain_scores_gemma":[0.99895144,0.000113213064,0.00035494813,0.00016097144,0.00015812043,0.00026126075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030198254,0.00018066684,0.0002003154,0.0016910512,0.00022576867,0.0007212706,0.0003322243,0.00015387767,0.001200245],"category_scores_gemma":[0.0012213918,0.00015883161,0.00023554376,0.0009719057,0.00017401937,0.0003466736,0.00078386517,0.00018839733,0.0003691312],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020253847,0.000036691403,0.9557521,0.000020216958,0.000075400036,0.0001446347,0.0002096472,0.0010559971,0.027709443,0.0002589657,0.001028412,0.013506108],"study_design_scores_gemma":[0.000003301949,0.000013440261,0.99738735,0.0000016618957,0.000007474955,0.000059658236,0.00002969148,0.0006303578,0.0012233998,0.000056738918,0.00058466964,0.0000022474899],"about_ca_topic_score_codex":0.010791122,"about_ca_topic_score_gemma":0.0154909305,"teacher_disagreement_score":0.010791122,"about_ca_system_score_codex":0.00025914836,"about_ca_system_score_gemma":0.00017989981,"threshold_uncertainty_score":0.0214566},"labels":[],"label_agreement":null},{"id":"W4389337175","doi":"10.3847/1538-4357/ad0968","title":"Magnetohydrodynamical Torsional Oscillations from Thermoresistive Instability in Hot Jupiters","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Instability; Hot Jupiter; Magnetic field; Oscillation (cell signaling); Thermal conduction; Mechanics; Astrophysics; Planet; Thermodynamics; Exoplanet","score_opus":0.011446586645023411,"score_gpt":0.22890237276029543,"score_spread":0.21745578611527203,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389337175","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99198407,0.00013268983,0.005088552,0.00012478569,0.000008315583,0.000009060901,0.000052958858,0.00009330262,0.0025062987],"genre_scores_gemma":[0.99937963,0.00003207695,0.00027489138,0.00000923913,0.000007302609,0.0000047373373,0.0000253339,0.000008276028,0.00025847083],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999633,0.000010070003,0.0000020193934,0.000007620856,0.000008889704,0.000008099998],"domain_scores_gemma":[0.99989533,0.000019089264,0.000045825007,0.00001196643,0.000009781601,0.000018089804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000787737,0.00043089627,0.0003112787,0.00021231874,0.0003058031,0.00055933604,0.00049594376,0.0005279203,0.0009415043],"category_scores_gemma":[0.0003765871,0.00020993553,0.0003710365,0.00015315645,0.0006063854,0.00040036408,0.0005509284,0.00028550078,0.0001167175],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022100244,0.00008692324,0.022885624,0.00011064891,0.00009355772,0.0012196891,0.00041093497,0.8534287,0.10123792,0.014155951,0.00080817635,0.005340783],"study_design_scores_gemma":[0.0000480448,0.00006769287,0.014861489,0.000005913437,0.000013502804,0.00012283504,0.0000446633,0.9776282,0.0021085343,0.004709815,0.00037289428,0.000016502712],"about_ca_topic_score_codex":0.0030029807,"about_ca_topic_score_gemma":0.0011490488,"teacher_disagreement_score":0.0030029807,"about_ca_system_score_codex":0.00044578427,"about_ca_system_score_gemma":0.00013080135,"threshold_uncertainty_score":0.005970955},"labels":[],"label_agreement":null},{"id":"W4389337235","doi":"10.3847/1538-4357/ad0971","title":"Diagnostics from Polarization of Scattered Optical Light from Galactic Infrared Cirrus","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Mount Allison University","funders":"","keywords":"Physics; Polarization (electrochemistry); Cosmic dust; Nebula; Scattering; Cirrus; Astrophysics; Rayleigh scattering; Mie scattering; Anisotropy; Sky; Optics; Infrared; Light scattering; Stars","score_opus":0.010718654157611831,"score_gpt":0.23242362930613203,"score_spread":0.2217049751485202,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389337235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9627028,0.00013323524,0.033566523,0.000051030347,0.000007333385,0.000010684246,0.00035068832,0.00020670427,0.0029709488],"genre_scores_gemma":[0.9971222,0.00003720916,0.002540011,0.000006953559,0.0000037119366,0.0000023466348,0.00018675046,0.000013266297,0.00008743157],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985087,0.00003955789,0.000005620313,0.000036020756,0.00004917278,0.000018696626],"domain_scores_gemma":[0.99939513,0.00019446765,0.00012893132,0.00011643021,0.000104367165,0.000060676288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003975222,0.00033109522,0.00015178794,0.00094026764,0.00014037352,0.0006585022,0.00024514593,0.0001865261,0.00052504404],"category_scores_gemma":[0.0012762928,0.00015460052,0.00029209626,0.0004375527,0.00027528018,0.00046380656,0.00033937246,0.00028246624,0.00013138336],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033264005,0.00005750802,0.6631265,0.00007483355,0.00021141952,0.0002734824,0.00015478185,0.15141836,0.13899392,0.009531066,0.0007211199,0.035104405],"study_design_scores_gemma":[0.00002575015,0.000099803525,0.33725697,0.0000281844,0.00004723052,0.00041015007,0.00015306832,0.6123228,0.04030062,0.0076894597,0.0016144197,0.000051579853],"about_ca_topic_score_codex":0.0021347874,"about_ca_topic_score_gemma":0.0017346694,"teacher_disagreement_score":0.0021347874,"about_ca_system_score_codex":0.00029875778,"about_ca_system_score_gemma":0.00013708929,"threshold_uncertainty_score":0.004244745},"labels":[],"label_agreement":null},{"id":"W4389390892","doi":"10.3847/1538-4357/ad077e","title":"SPLUS J142445.34–254247.1: An r-process–enhanced, Actinide-boost, Extremely Metal-poor Star Observed with GHOST","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Metallicity; Astrophysics; Stars; Supernova; Nucleosynthesis; Galactic halo; Thorium; Galaxy; Analytical Chemistry (journal); Uranium; Halo; Chemistry; Nuclear physics","score_opus":0.034888709537261656,"score_gpt":0.25607144939025217,"score_spread":0.22118273985299053,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389390892","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978331,0.000054788223,0.00016450572,0.000055623208,0.000009561255,0.000008634086,0.0003536164,0.00004575266,0.0014745474],"genre_scores_gemma":[0.9973611,0.000023347186,0.0005366126,0.00006836168,0.000014275305,0.0000068303325,0.0010174628,0.00002035337,0.00095158],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991536,0.0000050969047,0.0000038120575,0.000027137397,0.000025798801,0.00002282123],"domain_scores_gemma":[0.9997644,0.000012340937,0.000043603628,0.000018393992,0.000027784246,0.00013345243],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014289642,0.00043663126,0.00042139852,0.00084950746,0.00090273994,0.0004252797,0.000390217,0.00047340145,0.0016694061],"category_scores_gemma":[0.00019779551,0.00019568589,0.00022334523,0.00034964472,0.00035089458,0.0002244367,0.00063068385,0.00041537537,0.00087656995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010695228,0.00038749183,0.6705557,0.00013782427,0.00017525125,0.01528735,0.0007272848,0.0013229119,0.2825752,0.0007763599,0.005935753,0.021049364],"study_design_scores_gemma":[0.000047775295,0.0005097548,0.9714556,0.0000146172815,0.00003288537,0.004641541,0.0004595783,0.0018704857,0.012473586,0.00022182886,0.008242103,0.000030250876],"about_ca_topic_score_codex":0.0030598976,"about_ca_topic_score_gemma":0.0044468446,"teacher_disagreement_score":0.0030598976,"about_ca_system_score_codex":0.00042338198,"about_ca_system_score_gemma":0.00015537301,"threshold_uncertainty_score":0.006084144},"labels":[],"label_agreement":null},{"id":"W4389398001","doi":"10.3847/1538-4357/ad05c4","title":"X-Ray Polarization of the BL Lacertae Type Blazar 1ES 0229+200","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Consejo Superior de Investigaciones Científicas; Agencia Estatal de Investigación; Science Mission Directorate; Smithsonian Astrophysical Observatory; Instituto de Astrofísica de Andalucía; Istituto Nazionale di Fisica Nucleare; Goddard Space Flight Center; Universitetet i Oslo; Marshall Space Flight Center; Nuclear Safety and Security Commission; Háskóli Íslands; Istituto Nazionale di Astrofisica; Ministerio de Ciencia e Innovación; Junta de Andalucía; National Science Foundation; Agenzia Spaziale Italiana; Max-Planck-Gesellschaft; Centre National d’Etudes Spatiales; Academy of Finland; Horizon 2020 Framework Programme; Turun Yliopisto; Aarhus Universitet; Academia Sinica; National Aeronautics and Space Administration; Stockholms Universitet; Centre National de la Recherche Scientifique; Smithsonian Institution","keywords":"Blazar; Physics; Astrophysics; Polarization (electrochemistry); Synchrotron; Polarimetry; Position angle; Active galactic nucleus; Degree of polarization; Astronomy; Optics; Galaxy; Scattering; Gamma ray","score_opus":0.008781047909560673,"score_gpt":0.221215715082802,"score_spread":0.21243466717324133,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389398001","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996357,0.000055890767,0.00018133252,0.00003319722,0.0000034537177,0.0000033691367,0.00050621957,0.000039381408,0.0028200913],"genre_scores_gemma":[0.99831885,0.0000293229,0.0001603362,0.000026238544,0.0000066668376,0.0000032578669,0.0009494058,0.000009793684,0.000495976],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999409,0.000005943441,0.0000023211187,0.000019899615,0.00001688253,0.0000140603515],"domain_scores_gemma":[0.99983895,0.000023050985,0.000055096618,0.00001935435,0.000029474506,0.000034057077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012989427,0.00019048051,0.00013669507,0.00051467493,0.0001933228,0.00039930842,0.00016209124,0.00025305382,0.0017920339],"category_scores_gemma":[0.00024552745,0.000117934935,0.00010959989,0.00035299006,0.00013346136,0.00017766871,0.00024683858,0.00024743922,0.000530637],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00086913834,0.00018626465,0.4357849,0.00006511231,0.00008441787,0.001147174,0.00039206326,0.0014877098,0.54305154,0.0005321993,0.0019517355,0.014447689],"study_design_scores_gemma":[0.000012527392,0.000046171637,0.9921536,0.00000396474,0.000010083721,0.00022050945,0.00006448988,0.00082213193,0.0057686297,0.00005781663,0.00083353824,0.000006429267],"about_ca_topic_score_codex":0.0017158492,"about_ca_topic_score_gemma":0.002814918,"teacher_disagreement_score":0.0017920339,"about_ca_system_score_codex":0.00018306506,"about_ca_system_score_gemma":0.00005635657,"threshold_uncertainty_score":0.0059949756},"labels":[],"label_agreement":null},{"id":"W4389398114","doi":"10.3847/1538-4357/acfe75","title":"Characterizing the Near-infrared Spectra of Flares from TRAPPIST-1 during JWST Transit Spectroscopy Observations","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":52,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Herzberg Institute of Astrophysics; Université du Québec à Montréal; University of Victoria; Université de Montréal","funders":"Astrophysics Division; Science Mission Directorate; Space Telescope Science Institute","keywords":"Physics; Transit (satellite); Spectral line; Spectroscopy; Infrared spectroscopy; Infrared; Astronomy; Astrophysics; Astrobiology","score_opus":0.01900426758455524,"score_gpt":0.22575044726612226,"score_spread":0.20674617968156703,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389398114","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99828017,0.000038688715,0.00024793798,0.0000102922595,0.000003137214,0.000007689046,0.00045953647,0.00005600735,0.0008965711],"genre_scores_gemma":[0.9970818,0.000027840415,0.0006114142,0.000017720122,0.000006050325,0.000010017456,0.0016868081,0.000026722135,0.0005316939],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999918,0.000002955158,0.000002876358,0.000020690984,0.000034703797,0.000020835852],"domain_scores_gemma":[0.999723,0.000023475435,0.000085866464,0.000021041056,0.00007976645,0.000066914596],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000121212724,0.00020946427,0.00020411205,0.00084987463,0.00042830317,0.00029402022,0.00026388865,0.00022895398,0.0010229961],"category_scores_gemma":[0.00033622055,0.0001232758,0.00018773315,0.0005240891,0.00014242194,0.00025486763,0.00038569813,0.00031689068,0.00026735457],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048239643,0.00013538661,0.6401381,0.00009978918,0.0001385067,0.0010631812,0.00077939115,0.0011424302,0.33120102,0.000112676265,0.001465751,0.023241414],"study_design_scores_gemma":[0.0000050297635,0.00008608039,0.99225265,0.0000039864476,0.000017278235,0.00021825173,0.000089534886,0.0009060144,0.0055792513,0.00001399106,0.0008232423,0.000004688765],"about_ca_topic_score_codex":0.003211405,"about_ca_topic_score_gemma":0.010344834,"teacher_disagreement_score":0.003211405,"about_ca_system_score_codex":0.0002800315,"about_ca_system_score_gemma":0.000105455314,"threshold_uncertainty_score":0.0063854456},"labels":[],"label_agreement":null},{"id":"W4389453416","doi":"10.3847/1538-4357/ad022b","title":"JWST: Deuterated PAHs, PAH Nitriles, and PAH Overtone and Combination Bands. I. Program Description and First Look","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"Space Telescope Science Institute","keywords":"Overtone; Physics; Deuterium; Emission spectrum; Astrophysics; Polycyclic aromatic hydrocarbon; Spectral line; Analytical Chemistry (journal); Atomic physics; Astronomy; Chemistry; Astrobiology; Organic chemistry","score_opus":0.012402740059308633,"score_gpt":0.23422407542716278,"score_spread":0.22182133536785414,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389453416","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.45115513,0.0006092542,0.08895371,0.0008436012,0.00013615155,0.0009263489,0.22157642,0.18494081,0.050858576],"genre_scores_gemma":[0.39373812,0.00030252972,0.21514887,0.0005108873,0.00021820092,0.0010469495,0.3350632,0.02061507,0.03335623],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99980396,0.0000107372225,0.00000980643,0.00007130721,0.000068386995,0.00003578849],"domain_scores_gemma":[0.9995276,0.000077431825,0.00008811398,0.00009020268,0.00011279767,0.00010375792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004276306,0.00070682477,0.00030271875,0.0014879098,0.00041726566,0.0005815748,0.0008644348,0.0003092327,0.023311833],"category_scores_gemma":[0.00046670478,0.00042143968,0.0005710947,0.0012023109,0.00013883259,0.00065947796,0.0006108484,0.0004798259,0.006894469],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.004090929,0.0008237288,0.18857485,0.0009311843,0.00039790536,0.0007670002,0.0006298272,0.004266903,0.27443376,0.0016475165,0.15481615,0.3686202],"study_design_scores_gemma":[0.000643324,0.00084649434,0.49750152,0.000077707184,0.00018702031,0.00090041594,0.0002513995,0.0361389,0.24923468,0.0018625852,0.21217033,0.00018558491],"about_ca_topic_score_codex":0.0023587102,"about_ca_topic_score_gemma":0.0047731968,"teacher_disagreement_score":0.023311833,"about_ca_system_score_codex":0.00028071232,"about_ca_system_score_gemma":0.00023956895,"threshold_uncertainty_score":0.07798582},"labels":[],"label_agreement":null},{"id":"W4389562581","doi":"10.3847/1538-4357/aceefc","title":"A Search for IceCube Sub-TeV Neutrinos Correlated with Gravitational-wave Events Detected By LIGO/Virgo","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; National Research Foundation; Michigan State University; University of Oxford; Chiba University; Santen; Compute Canada; Marquette University","keywords":"Physics; Neutrino; LIGO; Astrophysics; Astronomy; Observatory; Gravitational wave; Neutrino detector; Neutrino astronomy; Population; Solar neutrino problem; Solar neutrino; Particle physics; Neutrino oscillation","score_opus":0.0128560873285582,"score_gpt":0.23582001963659943,"score_spread":0.22296393230804123,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389562581","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99412763,0.00010554613,0.0011174435,0.00005923555,0.000008547504,0.00002654552,0.0025172695,0.00007687811,0.001960962],"genre_scores_gemma":[0.98428255,0.00008683975,0.0042216443,0.000065512024,0.00003064294,0.00003717568,0.010437869,0.00003925374,0.0007985057],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99953747,0.00011365671,0.000022598108,0.00014139194,0.00011089887,0.0000739809],"domain_scores_gemma":[0.9980253,0.00085673615,0.0005389469,0.000164555,0.00016873611,0.0002457816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008972278,0.00032120405,0.00038862106,0.0018592275,0.00037920036,0.00089574105,0.00039205747,0.0003364413,0.0019004352],"category_scores_gemma":[0.002074094,0.00015596986,0.0003499595,0.0018693525,0.0002334065,0.0002843078,0.0007084409,0.0002541082,0.00031071357],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001835171,0.00019177461,0.9493362,0.00007721831,0.00029863993,0.0006259162,0.00019022597,0.0030082336,0.023646494,0.0010157278,0.0025132096,0.017261289],"study_design_scores_gemma":[0.00017611527,0.00039008807,0.95580345,0.000025236814,0.00018222534,0.0007810512,0.0002828618,0.01859964,0.016933594,0.0008095934,0.0059858607,0.000030133793],"about_ca_topic_score_codex":0.0037121028,"about_ca_topic_score_gemma":0.00569186,"teacher_disagreement_score":0.0037121028,"about_ca_system_score_codex":0.00036643198,"about_ca_system_score_gemma":0.0005250896,"threshold_uncertainty_score":0.007381022},"labels":[],"label_agreement":null},{"id":"W4389615828","doi":"10.3847/1538-4357/acfa6f","title":"High-sensitivity Beamformed Observations of the Crab Pulsar's Radio Emission","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Killam Trusts","keywords":"Physics; Crab Pulsar; Astrophysics; Pulsar; Flux (metallurgy); Crab Nebula; Pulse (music); Astronomy; Sensitivity (control systems); Optics; Detector","score_opus":0.02220379859051916,"score_gpt":0.3029038522975174,"score_spread":0.2807000537069982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389615828","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964155,0.00015779621,0.0012475763,0.000024189601,0.000004276973,0.00000740121,0.00120492,0.00007829513,0.0008599645],"genre_scores_gemma":[0.99588287,0.00004691985,0.0017508599,0.000020142503,0.0000121972425,0.000008708119,0.002072083,0.000019220457,0.00018700458],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978966,0.000046932622,0.000011124525,0.000052505635,0.000055801895,0.000044093827],"domain_scores_gemma":[0.99926645,0.00021657039,0.00017175578,0.00012304497,0.00012973094,0.00009245881],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059819396,0.00024880897,0.000250774,0.0015395435,0.0002218534,0.00050893065,0.00028477877,0.00029610755,0.00080544245],"category_scores_gemma":[0.0009776242,0.00027978758,0.0002894157,0.0009366294,0.00019635445,0.00026716245,0.00042747307,0.0002151639,0.0002818255],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045938994,0.00012644638,0.7760107,0.00007096511,0.00037026458,0.0005631744,0.00046075668,0.006621019,0.18854006,0.00039319362,0.0009014096,0.025482595],"study_design_scores_gemma":[0.000008679402,0.000025605015,0.99531156,0.000003872144,0.000018720493,0.00011366856,0.000018314879,0.0017627347,0.0021807344,0.000054026685,0.0004948086,0.0000074512577],"about_ca_topic_score_codex":0.0029691136,"about_ca_topic_score_gemma":0.0072878874,"teacher_disagreement_score":0.0029691136,"about_ca_system_score_codex":0.00032406833,"about_ca_system_score_gemma":0.00012568723,"threshold_uncertainty_score":0.0059036613},"labels":[],"label_agreement":null},{"id":"W4389615917","doi":"10.3847/1538-4357/acfc39","title":"The GBT Diffuse Ionized Gas Survey (GDIGS): Discrete Sources","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"European Southern Observatory; West Virginia University; National Science Foundation","keywords":"Physics; Galactic plane; Astrophysics; Ionization; Green Bank Telescope; Plasma; Line (geometry); Emission spectrum; Telescope; Galactic Center; Galaxy; Astronomy; Ion; Spectral line; Nuclear physics; Geometry","score_opus":0.016096711551843768,"score_gpt":0.2543292198440789,"score_spread":0.23823250829223513,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389615917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97909,0.0004514654,0.0016868429,0.00012245534,0.000009409804,0.000040552797,0.0127061205,0.0001703815,0.0057228957],"genre_scores_gemma":[0.9842196,0.00015171112,0.0019757736,0.000077269804,0.000015188188,0.00001782622,0.012814845,0.000025023326,0.0007028029],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985516,0.000011812012,0.0000070857036,0.000046903435,0.00004560471,0.000033460205],"domain_scores_gemma":[0.99962306,0.00003546559,0.00013455591,0.000050085044,0.000042371645,0.000114398645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019507876,0.00016679236,0.0001779678,0.0015697642,0.00024009607,0.00044885717,0.00032964855,0.00013369421,0.0014846326],"category_scores_gemma":[0.000352912,0.000084016305,0.00013649162,0.0019454976,0.00024720907,0.00022082038,0.00075658533,0.00020156208,0.00048273237],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012999924,0.00002974834,0.968073,0.000038237937,0.0000612279,0.0001788322,0.00026045775,0.0005810382,0.009185748,0.00054124685,0.0036371592,0.01728336],"study_design_scores_gemma":[0.000013869619,0.000014341487,0.9951835,0.000011553662,0.000013013046,0.00012620576,0.000117377385,0.0005039733,0.000599618,0.00019242484,0.0032217137,0.0000024795695],"about_ca_topic_score_codex":0.018804744,"about_ca_topic_score_gemma":0.02953309,"teacher_disagreement_score":0.018804744,"about_ca_system_score_codex":0.0003749534,"about_ca_system_score_gemma":0.0002495973,"threshold_uncertainty_score":0.03739053},"labels":[],"label_agreement":null},{"id":"W4389616026","doi":"10.3847/1538-4357/ad004d","title":"The Close AGN Reference Survey (CARS): An Interplay between Radio Jets and AGN Radiation in the Radio-quiet AGN HE0040-1105","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; University of Manitoba","funders":"Goddard Space Flight Center; National Science Foundation; Instituto de Astrofísica de Andalucía; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Agencia Estatal de Investigación; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Active galactic nucleus; Astronomy; Galaxy; Outflow; Radio galaxy; Accretion (finance); Star formation; Supermassive black hole; Very-long-baseline interferometry","score_opus":0.019410508374497752,"score_gpt":0.27390069407136336,"score_spread":0.2544901856968656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389616026","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989452,0.000054551256,0.00015710111,0.000019635792,0.0000013056896,0.000002899928,0.00011442589,0.000009058287,0.0006959612],"genre_scores_gemma":[0.99931026,0.000022817208,0.00025833581,0.000012704777,0.000004286695,0.0000013987128,0.0001922871,0.000002545282,0.00019539938],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965084,0.00006923558,0.000016622706,0.00011552263,0.00008610347,0.0000616722],"domain_scores_gemma":[0.99939084,0.00011440895,0.00022733609,0.00006128041,0.00007824164,0.00012789192],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044334988,0.00010182558,0.00012125723,0.0011234682,0.00027311247,0.00057500234,0.0003379108,0.00024791222,0.00061907584],"category_scores_gemma":[0.0009318064,0.00009843824,0.00012618235,0.0006177695,0.00027449627,0.00024298392,0.0006166174,0.000104450315,0.00011971485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012491684,0.0000410611,0.9746532,0.000017120601,0.000047725924,0.0012872249,0.00047826619,0.00045376306,0.010025946,0.00024773218,0.00035260952,0.0122704925],"study_design_scores_gemma":[0.0000040251234,0.000037532,0.9971674,0.0000038574503,0.000017969862,0.0005497412,0.00026059055,0.0008939355,0.00044514006,0.00003294024,0.00058087445,0.000005942656],"about_ca_topic_score_codex":0.015568731,"about_ca_topic_score_gemma":0.03321196,"teacher_disagreement_score":0.015568731,"about_ca_system_score_codex":0.00027447744,"about_ca_system_score_gemma":0.00014386822,"threshold_uncertainty_score":0.030956209},"labels":[],"label_agreement":null},{"id":"W4389687365","doi":"10.3847/1538-4357/ad0cc0","title":"All We Are Is Dust in the WIM: Constraints on Dust Properties in the Milky Way’s Warm Ionized Medium","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Athabasca University; University of Calgary; National Research Council Canada; Canadian Institute for Theoretical Astrophysics; Dominion Astrophysical Observatory; University of Toronto; Herzberg Institute of Astrophysics","funders":"NordForsk; University of Toronto; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; Royal Astronomical Society","keywords":"Physics; Milky Way; Ionization; Astrophysics; Analytical Chemistry (journal); Galaxy; Ion; Chemistry","score_opus":0.038511109157746165,"score_gpt":0.26010851203631785,"score_spread":0.2215974028785717,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389687365","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963361,0.00037555845,0.0004969916,0.000087260974,0.0000065624477,0.0000026494818,0.00026001848,0.000027888873,0.0024068807],"genre_scores_gemma":[0.99888426,0.00012413342,0.00031233305,0.00003509621,0.000009139054,0.0000026404123,0.00025377295,0.000010836928,0.00036786566],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998987,0.000010066635,0.0000057658553,0.000028709519,0.000028666209,0.000028203081],"domain_scores_gemma":[0.9996313,0.0000575042,0.00012762962,0.00005523473,0.00003833233,0.00008992635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001603269,0.00015486551,0.0002348347,0.0005823764,0.00035999686,0.0012525741,0.000266608,0.00020693049,0.0012701978],"category_scores_gemma":[0.0005757205,0.00013565343,0.000261028,0.00043251005,0.00033869693,0.0005494499,0.0007348092,0.00019043693,0.00028723283],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001729038,0.000030289571,0.9454825,0.00005747419,0.0001851062,0.00028609557,0.00049072894,0.001099888,0.030794496,0.0012533575,0.00094659696,0.019200655],"study_design_scores_gemma":[0.0000070482556,0.000036368972,0.988159,0.000016690487,0.000057304787,0.00011629096,0.00043447735,0.0011157376,0.0045405547,0.0004921311,0.005013188,0.000011238735],"about_ca_topic_score_codex":0.0068122465,"about_ca_topic_score_gemma":0.01634271,"teacher_disagreement_score":0.0068122465,"about_ca_system_score_codex":0.0003998343,"about_ca_system_score_gemma":0.0001578677,"threshold_uncertainty_score":0.013545215},"labels":[],"label_agreement":null},{"id":"W4389687367","doi":"10.3847/1538-4357/ad0ce9","title":"Electromagnetic Characterization of the LISA Verification Binary ZTF J0526+5934","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Planetary Science Division; Deutsches Elektronen-Synchrotron; Science and Technology Facilities Council; Science Mission Directorate; Stockholms Universitet; University of California, Los Angeles; Jet Propulsion Laboratory; Smithsonian Astrophysical Observatory; NASA Headquarters; Max-Planck-Institut für Astronomie; Gordon and Betty Moore Foundation; Queen's University Belfast; Queen's University; NASA Exoplanet Science Institute; Los Alamos National Laboratory; University of Washington; Johns Hopkins University; W. M. Keck Foundation; Space Telescope Science Institute; National Science Foundation; Texas Tech University; National Central University; Nuclear Safety and Security Commission; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Aeronautics and Space Administration; Natural Sciences and Engineering Research Council of Canada; Durham University; Smithsonian Institution","keywords":"Physics; White dwarf; Astrophysics; Astronomy; Binary number; Binary star; Subdwarf; Stars","score_opus":0.009029566638776344,"score_gpt":0.21482749157938447,"score_spread":0.2057979249406081,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389687367","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99732095,0.00004393213,0.0001903726,0.00002528786,0.000005803464,0.000008105157,0.00088041497,0.000025096884,0.0015000842],"genre_scores_gemma":[0.9959462,0.000016649612,0.0005190233,0.000014410659,0.000008184115,0.0000056043473,0.0027264091,0.0000067636993,0.0007567944],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998517,0.000009631846,0.000008784921,0.000033996243,0.00005359813,0.00004223173],"domain_scores_gemma":[0.99944,0.000046140147,0.00020278117,0.000049433882,0.00013693776,0.00012475342],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023001844,0.0001436437,0.00024982207,0.0017165918,0.0006532572,0.00042998593,0.00026015914,0.00022923794,0.0018462436],"category_scores_gemma":[0.00057755393,0.00012523383,0.000120327706,0.0010974722,0.00017003722,0.00019476893,0.00036005382,0.0002238855,0.00058750855],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00090523274,0.00027609646,0.85018855,0.000050125534,0.000037986494,0.0014960049,0.00047061715,0.0010971638,0.113046564,0.00089471246,0.0022733829,0.029263662],"study_design_scores_gemma":[0.000010407912,0.00008844701,0.9931003,0.000003854407,0.0000072062153,0.00036005952,0.00010851759,0.0012304861,0.0026944357,0.00006794531,0.002319808,0.00000859743],"about_ca_topic_score_codex":0.007861235,"about_ca_topic_score_gemma":0.01529861,"teacher_disagreement_score":0.007861235,"about_ca_system_score_codex":0.0005351823,"about_ca_system_score_gemma":0.0002323175,"threshold_uncertainty_score":0.01563096},"labels":[],"label_agreement":null},{"id":"W4389735300","doi":"10.3847/1538-4357/ad0640","title":"Origin of High-velocity Ejecta, Excess Emission, and Redward Color Evolution in the Infant Type Ia Supernova 2021aefx","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Ejecta; Physics; Astrophysics; Supernova; Photosphere; Photometry (optics); Astronomy; Type II supernova; Spectral line; Stars","score_opus":0.013464848662829137,"score_gpt":0.26064359262191444,"score_spread":0.24717874395908532,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389735300","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99940586,0.000080005615,0.00008066402,0.000005270293,0.0000010045609,0.000002509378,0.00010006655,0.0000063177695,0.00031831214],"genre_scores_gemma":[0.99918956,0.000051704792,0.00013965368,0.000005624561,0.0000022448914,0.0000023349123,0.0003611787,0.0000035262983,0.00024403393],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999397,0.0000056861572,0.000004441682,0.000019274972,0.00001560012,0.000015369442],"domain_scores_gemma":[0.9997559,0.00002887926,0.0000932401,0.000015224687,0.000028659846,0.00007817988],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019288276,0.00029636823,0.00018250213,0.00078513037,0.00021019892,0.0004302746,0.00016186883,0.00020741326,0.0010488405],"category_scores_gemma":[0.0003863522,0.00013618481,0.0001965811,0.00021700124,0.00016541412,0.00013325218,0.00031218486,0.00017901893,0.00022217198],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024373012,0.0000460835,0.9524088,0.000015678821,0.000024018802,0.0013744354,0.0001021795,0.00021280242,0.040916283,0.00012622586,0.00008867042,0.0044411216],"study_design_scores_gemma":[7.859311e-7,0.00003085021,0.99795157,0.0000020146083,0.0000032762937,0.0007308908,0.000027125048,0.00014426689,0.0009786697,0.000013824132,0.00011524357,0.0000015000882],"about_ca_topic_score_codex":0.0032223293,"about_ca_topic_score_gemma":0.0028264339,"teacher_disagreement_score":0.0032223293,"about_ca_system_score_codex":0.00025177613,"about_ca_system_score_gemma":0.00009028607,"threshold_uncertainty_score":0.0064071417},"labels":[],"label_agreement":null},{"id":"W4389763626","doi":"10.3847/1538-4357/ace5a3","title":"Stellar Properties of Observed Stars Stripped in Binaries in the Magellanic Clouds","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":66,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Space Telescope Science Institute; National Aeronautics and Space Administration; Canada Research Chairs; Canadian Institute for Advanced Research; University of Toronto","keywords":"Physics; Stars; Astrophysics; Large Magellanic Cloud; Astronomy; Stellar collision; Stellar evolution","score_opus":0.03790950938928171,"score_gpt":0.23026386582556038,"score_spread":0.19235435643627868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389763626","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99947554,0.000044849734,0.000100070465,0.0000050819685,0.0000014951864,0.0000013580074,0.00019367131,0.000011825749,0.00016611432],"genre_scores_gemma":[0.9994172,0.000011581897,0.00006382954,0.0000032973414,0.0000013602987,7.5086587e-7,0.00041422332,0.0000036615106,0.00008406076],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999075,0.000011221003,0.000008212131,0.000029262706,0.000018953826,0.000024790023],"domain_scores_gemma":[0.99958795,0.00009195856,0.00008980076,0.00003558468,0.00006077,0.00013392516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002628674,0.00026296993,0.00023144575,0.00091987924,0.0003316123,0.00051874015,0.00025806646,0.0004081635,0.0010743036],"category_scores_gemma":[0.0005911449,0.00013052375,0.00026592182,0.000672815,0.00021690155,0.0003286275,0.00036985555,0.00022322175,0.00037542928],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002805086,0.000050530587,0.97699374,0.00002262902,0.00009042566,0.00015013355,0.00018141957,0.0023620212,0.01631591,0.00010361274,0.00013561083,0.0033133763],"study_design_scores_gemma":[0.0000052059772,0.00003764467,0.99154985,0.0000026853997,0.000015573765,0.00011182238,0.000113068236,0.0054677036,0.002427104,0.00006270502,0.00020073721,0.0000058492024],"about_ca_topic_score_codex":0.004269035,"about_ca_topic_score_gemma":0.002875879,"teacher_disagreement_score":0.004269035,"about_ca_system_score_codex":0.00043365234,"about_ca_system_score_gemma":0.00008282926,"threshold_uncertainty_score":0.008488357},"labels":[],"label_agreement":null},{"id":"W4389893104","doi":"10.3847/1538-4357/ad0842","title":"First X-Ray Polarization Measurement Confirms the Low Black Hole Spin in LMC X-3","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Agenzia Spaziale Italiana; Nuclear Safety and Security Commission; Centre National d’Etudes Spatiales; Grantová Agentura České Republiky; University of Leicester; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Black hole (networking); Polarization (electrochemistry); Polarimetry; X-ray binary; Large Magellanic Cloud; X-ray; Astronomy; Stars; Neutron star; Scattering; Optics","score_opus":0.02331355884815282,"score_gpt":0.2375449745656055,"score_spread":0.2142314157174527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389893104","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808407,0.00006346034,0.0004330648,0.000029122228,0.0000049520318,0.000006180478,0.0002077517,0.000028103319,0.0011433298],"genre_scores_gemma":[0.99928373,0.000016971957,0.00031958628,0.000023699258,0.0000057768243,0.000003179683,0.00021952906,0.000008037563,0.0001195134],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998534,0.000011959311,0.0000066891253,0.00004206495,0.000037961658,0.000048047696],"domain_scores_gemma":[0.9997396,0.000031313266,0.00007926371,0.000039422663,0.00005544666,0.000054994132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017293924,0.0002864021,0.00024185899,0.0007090617,0.0006860338,0.00062214007,0.00020726421,0.0004579504,0.001159903],"category_scores_gemma":[0.00029005215,0.00011333786,0.00019776722,0.00047718678,0.0004380489,0.00018273004,0.0005056565,0.00044051808,0.00034473505],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038735487,0.00007306439,0.4946968,0.00003644577,0.000047985937,0.0016958681,0.00041608667,0.00018566233,0.49555007,0.0002939669,0.0005448485,0.0060718977],"study_design_scores_gemma":[0.000010208438,0.00007505106,0.95634055,0.000006869646,0.000019976287,0.0012084531,0.00018072502,0.00074928196,0.04032614,0.000111537,0.000963461,0.000007806401],"about_ca_topic_score_codex":0.0023232077,"about_ca_topic_score_gemma":0.0023908278,"teacher_disagreement_score":0.0023232077,"about_ca_system_score_codex":0.00025450144,"about_ca_system_score_gemma":0.00011420218,"threshold_uncertainty_score":0.00461936},"labels":[],"label_agreement":null},{"id":"W4389979069","doi":"10.3847/1538-4357/ad0153","title":"Strong Carbon Features and a Red Early Color in the Underluminous Type Ia SN 2022xkq","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"European Social Fund; Agencia Estatal de Investigación; Consejo Superior de Investigaciones Científicas; Japan Society for the Promotion of Science; Science and Technology Facilities Council; University of North Carolina at Chapel Hill; Agencia Nacional de Investigación y Desarrollo; Astrophysics Division; Istituto Nazionale di Astrofisica; Centre National de la Recherche Scientifique; Nuclear Safety and Security Commission; Ministério da Ciência, Tecnologia e Inovação; Commonwealth Scientific and Industrial Research Organisation; Queen's University Belfast; Australian Government; Heising-Simons Foundation; Space Telescope Science Institute; Vetenskapsrådet; Smithsonian Institution; John Templeton Foundation; National Natural Science Foundation of China; Arizona Board of Regents; Leibniz-Gemeinschaft; University of Notre Dame; Queen's University; Jet Propulsion Laboratory; Leibniz-Institut für Astrophysik Potsdam; University of California, Santa Cruz; Ohio State University; National Science Foundation; University of Minnesota; Centre National d’Etudes Spatiales; Aspen Center for Physics; College of Engineering, Michigan State University; Università degli Studi di Padova; Ministero dell’Istruzione, dell’Università e della Ricerca; Alfred P. Sloan Foundation; Ministerio de Ciencia e Innovación; European Commission; Precursory Research for Embryonic Science and Technology; California Institute of Technology; National Aeronautics and Space Administration; Michigan State University","keywords":"Physics; Supernova; Astrophysics; Light curve; White dwarf; Pair-instability supernova; Spectral line; Astronomy; Infrared; Ejecta; Stars","score_opus":0.014865548115293776,"score_gpt":0.2516261483978184,"score_spread":0.2367606002825246,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4389979069","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990012,0.000043518226,0.000118264354,0.000013542617,0.000003254465,0.0000034036673,0.00013172258,0.000010422465,0.0006748088],"genre_scores_gemma":[0.9989471,0.000025403628,0.00016511037,0.00002300667,0.0000059414656,0.000004291034,0.00040466746,0.0000043551013,0.00042011816],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999466,0.0000042552892,0.0000030635672,0.000014087706,0.000015034748,0.000016965747],"domain_scores_gemma":[0.9997842,0.000015582365,0.00007288943,0.000015050122,0.000029835013,0.000082425046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015206871,0.00029397986,0.00019202307,0.0007836023,0.0003041931,0.0003891959,0.00018992917,0.00027705613,0.001084636],"category_scores_gemma":[0.00018883833,0.00016030979,0.00018476642,0.0002444103,0.00030184494,0.00017381921,0.00038190323,0.00029754968,0.00036254685],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046267288,0.00015087806,0.81753826,0.000041189076,0.00006262169,0.0025397902,0.000427499,0.00046812426,0.17156944,0.00027153234,0.00064764736,0.005820466],"study_design_scores_gemma":[0.000004114411,0.00008431309,0.99772185,0.0000028955149,0.0000047550675,0.00036022143,0.00009359838,0.00016161558,0.0010794308,0.000037647176,0.0004458812,0.000003666052],"about_ca_topic_score_codex":0.0037570123,"about_ca_topic_score_gemma":0.0067130965,"teacher_disagreement_score":0.0037570123,"about_ca_system_score_codex":0.0002467574,"about_ca_system_score_gemma":0.000065110384,"threshold_uncertainty_score":0.00747025},"labels":[],"label_agreement":null},{"id":"W4390051172","doi":"10.3847/1538-4357/ad05c9","title":"Orbital Decay of Hot Jupiters due to Weakly Nonlinear Tidal Dissipation","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"California Institute of Technology; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Hot Jupiter; Subgiant; Astrophysics; Orbital decay; Stars; Dissipation; Tidal acceleration; Planetary system; Planet; Jupiter (rocket family); Astronomy; Exoplanet; Quantum mechanics","score_opus":0.011749543550691494,"score_gpt":0.2445181734531455,"score_spread":0.232768629902454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390051172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989147,0.000018823543,0.00033535046,0.000022922812,0.000002377517,0.0000024893645,0.000029391877,0.000019103,0.000654815],"genre_scores_gemma":[0.99948573,0.000013409889,0.0001801402,0.000009584995,0.0000019274405,0.000002950986,0.000039851613,0.000008252599,0.00025814548],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999435,0.000010612387,0.0000022951992,0.000009057228,0.000011056668,0.000023505638],"domain_scores_gemma":[0.9996412,0.00012703889,0.00008905519,0.000027270711,0.000033417808,0.00008207952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021682771,0.0003028039,0.00029092593,0.0003196025,0.0005192084,0.0006308477,0.00054286496,0.00054860633,0.0014152572],"category_scores_gemma":[0.0010960768,0.00020649098,0.0005114736,0.00024288315,0.00069932017,0.00038100194,0.0004992654,0.00047120402,0.000120585],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004621199,0.00016608178,0.10256876,0.000056736513,0.00013184604,0.0010871139,0.00037773984,0.86820996,0.019438282,0.0028255938,0.0005489919,0.0041268193],"study_design_scores_gemma":[0.00009546762,0.00030550337,0.0500308,0.000014258895,0.0000471815,0.0001365238,0.00018375403,0.9440195,0.003887527,0.00085908413,0.00039965985,0.000020691816],"about_ca_topic_score_codex":0.0077460385,"about_ca_topic_score_gemma":0.0044928975,"teacher_disagreement_score":0.0077460385,"about_ca_system_score_codex":0.0006244024,"about_ca_system_score_gemma":0.0002690884,"threshold_uncertainty_score":0.0154019},"labels":[],"label_agreement":null},{"id":"W4390051371","doi":"10.3847/1538-4357/ad0786","title":"ALMA-IMF. IX. Catalog and Physical Properties of 315 SiO Outflow Candidates in 15 Massive Protoclusters","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Key Research and Development Program of China; Japan Society for the Promotion of Science; Agence Nationale de la Recherche; Universidad Nacional Autónoma de México; National Natural Science Foundation of China; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Outflow; Astrophysics; Astronomy; Meteorology","score_opus":0.011991680573862996,"score_gpt":0.22013270263365947,"score_spread":0.20814102205979648,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390051371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9828644,0.00018416862,0.0005746407,0.00004412222,0.0000049135665,0.00006860765,0.010303139,0.0006069071,0.005349099],"genre_scores_gemma":[0.95630574,0.00013608833,0.0037104452,0.0000698496,0.000030649193,0.0001002561,0.03540964,0.000093497445,0.0041438527],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986756,0.00001337893,0.000010188371,0.000032594144,0.000038802486,0.000037489415],"domain_scores_gemma":[0.9993986,0.000072642004,0.00019649419,0.00007436721,0.000076282966,0.00018174041],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003841976,0.00034620063,0.00018218048,0.0028535123,0.00038577188,0.0004636885,0.00030307972,0.00012132628,0.0036119025],"category_scores_gemma":[0.0005880239,0.00012648483,0.00031659775,0.000928063,0.00012652199,0.00025104888,0.00059147854,0.00010675219,0.001321184],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004910213,0.00011232233,0.9420016,0.000052121875,0.00004741453,0.00041203573,0.00022759344,0.00043235038,0.010756902,0.00025167636,0.0071984287,0.03801643],"study_design_scores_gemma":[0.000031010608,0.00009105064,0.9872679,0.000008019929,0.000023803772,0.0002668879,0.00007931951,0.001467928,0.0025827677,0.00006681404,0.008107169,0.00000731368],"about_ca_topic_score_codex":0.004726525,"about_ca_topic_score_gemma":0.009216892,"teacher_disagreement_score":0.004726525,"about_ca_system_score_codex":0.00032408992,"about_ca_system_score_gemma":0.0002636299,"threshold_uncertainty_score":0.012082994},"labels":[],"label_agreement":null},{"id":"W4390058697","doi":"10.3847/1538-4357/ad02ee","title":"Stellar Half-mass Radii of 0.5 z &lt; 2.3 Galaxies: Comparison with JWST/NIRCam Half-light Radii","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Vlaamse regering; Fonds Wetenschappelijk Onderzoek","keywords":"Physics; Algorithm; Computer science","score_opus":0.009363306520187945,"score_gpt":0.2193749561847603,"score_spread":0.21001164966457236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390058697","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9883768,0.0003306184,0.0019156152,0.00006043969,0.000007690876,0.0000072540865,0.0015196718,0.0005801903,0.007201752],"genre_scores_gemma":[0.9959865,0.00004680589,0.00082023605,0.000030661384,0.000010617755,0.0000053633157,0.002127635,0.00009312387,0.000879081],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977833,0.000016628788,0.000010127674,0.00007238781,0.00006156072,0.000060909406],"domain_scores_gemma":[0.9989685,0.000097196906,0.00028217275,0.0001797788,0.00024523636,0.00022722744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047466965,0.00025748348,0.00023697733,0.0016394671,0.0002763736,0.0007620372,0.0006005352,0.00031478767,0.0020282797],"category_scores_gemma":[0.0010052549,0.00029019653,0.000458933,0.0006133395,0.00027169107,0.0004949324,0.0004764085,0.00024677647,0.001473106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036926442,0.00005651896,0.9041548,0.00008457389,0.0001325367,0.00017895484,0.00076620054,0.0028409844,0.056456354,0.0014558135,0.0042189225,0.029284986],"study_design_scores_gemma":[0.000005766594,0.000013800752,0.9891445,0.0000050523267,0.000017006034,0.00006486113,0.00007656325,0.0028282276,0.005948088,0.00013042668,0.0017571745,0.000008600209],"about_ca_topic_score_codex":0.007121985,"about_ca_topic_score_gemma":0.0063121836,"teacher_disagreement_score":0.007121985,"about_ca_system_score_codex":0.00053517264,"about_ca_system_score_gemma":0.00010991324,"threshold_uncertainty_score":0.01416105},"labels":[],"label_agreement":null},{"id":"W4390267295","doi":"10.3847/1538-4357/ad0120","title":"A Multiwavelength Investigation of PSR J2229+6114 and its Pulsar Wind Nebula in the Radio, X-Ray, and Gamma-Ray Bands","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; McGill University; University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; Office of Science; National Aeronautics and Space Administration; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Physics; Pulsar wind nebula; Astrophysics; Pulsar; Supernova remnant; Nebula; Fermi Gamma-ray Space Telescope; Astronomy; Supernova; Spectral energy distribution; Flux (metallurgy); Synchrotron; Stars; Galaxy","score_opus":0.012802683026560095,"score_gpt":0.2268196863341014,"score_spread":0.2140170033075413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390267295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99912196,0.00016601772,0.0001594407,0.000013252753,0.0000031384375,0.000004472465,0.00010380269,0.000011504982,0.00041653542],"genre_scores_gemma":[0.9986998,0.00009653823,0.0005280916,0.000016775813,0.000011210764,0.000004524895,0.00036562193,0.000007800028,0.00026962574],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991775,0.000006474323,0.0000059438707,0.00003088079,0.000020904872,0.000018094785],"domain_scores_gemma":[0.99977714,0.000018997443,0.00007727298,0.000018467048,0.000028559665,0.00007957898],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016988213,0.0002528963,0.00030139464,0.0013973928,0.0004191108,0.00030906708,0.00019211517,0.00020167933,0.0004683015],"category_scores_gemma":[0.00016216638,0.0001739371,0.00026194844,0.0006829678,0.00014839577,0.000255137,0.0005131569,0.00020959292,0.00018975162],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002662158,0.00017426006,0.7864299,0.00007051958,0.00017450452,0.0025010938,0.0005086019,0.0006388314,0.1893309,0.00017181612,0.00034737596,0.019385967],"study_design_scores_gemma":[0.0000044730946,0.00007094419,0.9969867,0.0000035829898,0.000020349571,0.00047042753,0.000099164965,0.00037685095,0.0013857656,0.000028760729,0.0005482903,0.0000047218764],"about_ca_topic_score_codex":0.0019449708,"about_ca_topic_score_gemma":0.0057236818,"teacher_disagreement_score":0.0019449708,"about_ca_system_score_codex":0.00015751914,"about_ca_system_score_gemma":0.000114860515,"threshold_uncertainty_score":0.0038672686},"labels":[],"label_agreement":null},{"id":"W4390341632","doi":"10.3847/1538-4357/ad0ecd","title":"X-Ray Characterization of the Pulsar PSR J1849−0001 and Its Wind Nebula G32.64+0.53 Associated with TeV Sources Detected by H.E.S.S., HAWC, Tibet ASγ, and LHAASO","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Pulsar wind nebula; Astrophysics; Pulsar; Spectral index; Nebula; Astronomy; Spectral line; Stars","score_opus":0.007497507751720417,"score_gpt":0.25153058696758496,"score_spread":0.24403307921586453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390341632","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989466,0.000042626016,0.00015690744,0.000008565992,0.0000015303473,0.000004588173,0.00017849989,0.000011954881,0.00064859766],"genre_scores_gemma":[0.9986357,0.000038870054,0.00027890413,0.000011153441,0.0000058647183,0.000005270694,0.0007822194,0.0000090215535,0.00023301713],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999449,0.000006478044,0.0000029090045,0.000016820886,0.000017687951,0.000011298417],"domain_scores_gemma":[0.9997851,0.000039647744,0.000085267755,0.000019297813,0.000030433672,0.000040329218],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018950227,0.00028203998,0.0002744688,0.00089120696,0.00029056915,0.00035387673,0.00019836324,0.00022000853,0.00088438473],"category_scores_gemma":[0.00028032268,0.00016410986,0.00017551883,0.00052636844,0.00018123032,0.00016381952,0.00028829402,0.00025804382,0.00018863802],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003710031,0.00018124002,0.8642221,0.000061216386,0.00007676337,0.0014893314,0.0002571691,0.0013916267,0.11629853,0.00024338323,0.00041675565,0.014990953],"study_design_scores_gemma":[0.000006910699,0.00007224233,0.99579644,0.0000037970426,0.000010485251,0.00032938196,0.000049843708,0.0011829196,0.0020043512,0.00003591077,0.0005042892,0.0000034503164],"about_ca_topic_score_codex":0.0012737875,"about_ca_topic_score_gemma":0.0021054107,"teacher_disagreement_score":0.0012737875,"about_ca_system_score_codex":0.00019486182,"about_ca_system_score_gemma":0.00007761024,"threshold_uncertainty_score":0.0029585361},"labels":[],"label_agreement":null},{"id":"W4390398168","doi":"10.3847/1538-4357/ad0559","title":"Disentangling Stellar Age Estimates from Galactic Chemodynamical Evolution","year":2023,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Milky Way; Astrophysics; Metallicity; Chemical evolution; Stars; Galaxy; Stellar evolution; Galaxy formation and evolution; Astronomy","score_opus":0.011266873383271979,"score_gpt":0.2331210138269513,"score_spread":0.22185414044367932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390398168","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9543921,0.00009596727,0.043266207,0.00021704951,0.000008209545,0.000008893268,0.00028458715,0.00007700737,0.001649993],"genre_scores_gemma":[0.99764663,0.000016736703,0.002151125,0.000015809435,0.0000035197754,0.0000014974945,0.000089508656,0.0000071720538,0.000067915396],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99924743,0.00031708743,0.000045082834,0.00022159502,0.00013102578,0.000037905054],"domain_scores_gemma":[0.9881627,0.007587199,0.001813673,0.0015266774,0.00064804044,0.00026174422],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038690525,0.00031398502,0.00031577388,0.00085579464,0.00025709614,0.0017921577,0.00067504717,0.0005827456,0.0009352272],"category_scores_gemma":[0.020240162,0.0002940614,0.00035451373,0.0005667134,0.0006572602,0.0017988775,0.001009788,0.0005858755,0.00018052994],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009251599,0.000029568615,0.87280613,0.000035569446,0.00019402198,0.00007566094,0.00027477957,0.09380471,0.0037054636,0.014386596,0.00022171556,0.0143733015],"study_design_scores_gemma":[0.000019016657,0.00007316051,0.2797314,0.000025054562,0.00007599673,0.00013283473,0.00020514519,0.67670816,0.0053534335,0.036450244,0.0011892283,0.000036313988],"about_ca_topic_score_codex":0.0023865825,"about_ca_topic_score_gemma":0.0031083552,"teacher_disagreement_score":0.0038690525,"about_ca_system_score_codex":0.00042274335,"about_ca_system_score_gemma":0.00026227257,"threshold_uncertainty_score":0.020461798},"labels":[],"label_agreement":null},{"id":"W4390701566","doi":"10.3847/1538-4357/ad1184","title":"Modeling Current and Future High-cadence Surveys of Repeating Fast Radio Burst Populations","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Science Foundation","keywords":"Physics; Redshift; Fast radio burst; Poisson distribution; Repeater (horology); Cadence; Population; Astrophysics; Sky; Monte Carlo method; Astronomy; Statistics; Computer science; Galaxy; Acoustics","score_opus":0.026477537187438487,"score_gpt":0.3426111194973596,"score_spread":0.3161335823099211,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390701566","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98801047,0.000052521442,0.010485797,0.00012798504,0.0000034190452,0.000029348705,0.00042865833,0.000093982155,0.00076778786],"genre_scores_gemma":[0.9954478,0.000047151792,0.0034674047,0.000029432054,0.000003350996,0.000024904923,0.00054067327,0.000017965685,0.0004212953],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996455,0.00008951794,0.000011038224,0.00013857381,0.00004719694,0.000068114125],"domain_scores_gemma":[0.99720395,0.0014078158,0.0005187406,0.00027765404,0.00032033856,0.000271445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019744027,0.00029672447,0.00033625436,0.00068194664,0.0005633579,0.0010139477,0.0015271911,0.0009819064,0.0011074761],"category_scores_gemma":[0.0063935895,0.000525215,0.0005824754,0.000701648,0.00096125,0.0012748168,0.0005274065,0.0005483844,0.00022981613],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008555971,0.00005357525,0.19337374,0.000020360952,0.00007606914,0.00011626092,0.00015641037,0.79779875,0.001108569,0.00369409,0.0004090623,0.0031075452],"study_design_scores_gemma":[0.000020503985,0.000040485767,0.03996831,0.000006024557,0.00001842082,0.000055992932,0.000060825852,0.95744824,0.00038115302,0.0016638795,0.00031826456,0.000017890614],"about_ca_topic_score_codex":0.10722791,"about_ca_topic_score_gemma":0.07296832,"teacher_disagreement_score":0.10722791,"about_ca_system_score_codex":0.0029427246,"about_ca_system_score_gemma":0.0010701804,"threshold_uncertainty_score":0.21320754},"labels":[],"label_agreement":null},{"id":"W4390747909","doi":"10.3847/1538-4357/ad0fe2","title":"Tomographic Imaging of the Sagittarius Spiral Arm's Magnetic Field Structure","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec; Queen's University","funders":"Japan Society for the Promotion of Science; European Space Agency","keywords":"Physics; Galactic plane; Molecular cloud; Sagittarius A*; Astrophysics; Sagittarius; Spiral galaxy; Galactic Center; Line-of-sight; Astronomy; Stars; Milky Way","score_opus":0.0047389087449760375,"score_gpt":0.20699050612728884,"score_spread":0.2022515973823128,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390747909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97541577,0.000550174,0.009893193,0.00026284682,0.00001660421,0.00005347406,0.0036799847,0.0007631511,0.009364704],"genre_scores_gemma":[0.9774136,0.0002834455,0.018679753,0.00007074666,0.000030560892,0.000019545303,0.0023475692,0.000107984466,0.0010469432],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999591,0.0000032142216,0.000001555521,0.000009125283,0.000016375194,0.000010677025],"domain_scores_gemma":[0.9998367,0.00002596525,0.000030008056,0.000017913126,0.00005261106,0.000036855206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010366039,0.0001881837,0.00015027681,0.0014948088,0.00015236042,0.0004424017,0.00018201483,0.00021993682,0.0025851869],"category_scores_gemma":[0.00025037932,0.0001830305,0.00014819046,0.0009283977,0.00012281937,0.0002467127,0.00026289347,0.00022835116,0.00046014643],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047657953,0.00013902069,0.112724505,0.00025420045,0.00014933816,0.001173028,0.0004433677,0.007729068,0.7980518,0.00078950997,0.0041336766,0.07393593],"study_design_scores_gemma":[0.00007490683,0.00020670964,0.8820125,0.00008382626,0.0001633906,0.0029384643,0.00061167876,0.044944894,0.05920988,0.00064519834,0.009055649,0.000052906787],"about_ca_topic_score_codex":0.0036244206,"about_ca_topic_score_gemma":0.007127847,"teacher_disagreement_score":0.0036244206,"about_ca_system_score_codex":0.0002729581,"about_ca_system_score_gemma":0.00023006056,"threshold_uncertainty_score":0.008648276},"labels":[],"label_agreement":null},{"id":"W4390750257","doi":"10.3847/1538-4357/ad0835","title":"Dual-band Observations of the Asymmetric Ring around CIDA 9A: Dead or Alive?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; HORIZON EUROPE Framework Programme; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Astronomical Observatory of Japan; European Commission; Korea Astronomy and Space Science Institute; Ministry of Education; National Aeronautics and Space Administration; Fondazione Cariplo; National Natural Science Foundation of China; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Protoplanet; Millimeter; Astrophysics; Submillimeter Array; Asymmetry; Wavelength; Planet; Circumstellar dust; Protoplanetary disk; Astronomy; Interplanetary dust cloud; Star formation; Cosmic dust; Solar System; Stars; Optics","score_opus":0.028991247722522186,"score_gpt":0.2640089338295685,"score_spread":0.23501768610704635,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390750257","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99700516,0.00012697764,0.0007158815,0.000069098525,0.00002595013,0.0000051221205,0.00039670698,0.000067299115,0.0015879065],"genre_scores_gemma":[0.99874675,0.000020540092,0.0008357834,0.000034273125,0.000015301253,0.0000029834328,0.000182128,0.000004778204,0.0001572721],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999143,0.0000058041123,0.0000034414538,0.00003681416,0.000018462677,0.000021169139],"domain_scores_gemma":[0.99965036,0.000034002856,0.00011163161,0.000041103216,0.000045660767,0.00011718534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017235335,0.00014022115,0.0002332746,0.0005429762,0.00035949182,0.000347786,0.00034757188,0.0002957543,0.0012528534],"category_scores_gemma":[0.0002610066,0.00014859968,0.00017961477,0.00024691204,0.00019936838,0.00019868351,0.0003889574,0.00041129172,0.0003610644],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009196632,0.00015838844,0.4602278,0.000101304046,0.00012080025,0.0008628871,0.00023911028,0.00041973527,0.51920384,0.0006373508,0.0017689193,0.015340296],"study_design_scores_gemma":[0.000045802997,0.000120992394,0.97806954,0.0000104163955,0.00004779643,0.000828945,0.00019253901,0.0014957727,0.016245171,0.00027398032,0.002652681,0.00001640405],"about_ca_topic_score_codex":0.0006114906,"about_ca_topic_score_gemma":0.0014179001,"teacher_disagreement_score":0.0012528534,"about_ca_system_score_codex":0.000196048,"about_ca_system_score_gemma":0.000065985914,"threshold_uncertainty_score":0.00419122},"labels":[],"label_agreement":null},{"id":"W4390750280","doi":"10.3847/1538-4357/ad055a","title":"Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations. I. Unique Galaxy Morphologies in Imaging","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Bishop's University","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs","keywords":"Physics; Astrophysics; Galaxy; Galaxy merger; Astronomy; Gravitational wave; Stellar mass; Galaxy formation and evolution; Star formation","score_opus":0.008726075577436262,"score_gpt":0.2340376841304615,"score_spread":0.22531160855302523,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390750280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998754,0.000030633808,0.000627518,0.000013923761,0.0000012766496,0.0000051556403,0.00025676173,0.00007030838,0.00024041692],"genre_scores_gemma":[0.9977023,0.000013818281,0.0014789669,0.0000063567268,0.0000023625012,0.0000038738417,0.0007179651,0.00002024366,0.000054156146],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988985,0.00002833723,0.0000074044,0.00003272094,0.00002487375,0.00001677101],"domain_scores_gemma":[0.99955755,0.0001276061,0.00013424027,0.000063859385,0.000033196862,0.00008347219],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035064813,0.00044057542,0.000230374,0.0008922007,0.00022128936,0.00046139382,0.00047097387,0.00028739692,0.0005100508],"category_scores_gemma":[0.001132979,0.0002067524,0.0005350803,0.00042911724,0.0002194818,0.00024171281,0.00054928515,0.00015934996,0.000101987775],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010709568,0.00023234269,0.6477684,0.000149212,0.00057410245,0.0005850048,0.00035505212,0.21553276,0.107233174,0.0015553111,0.0007751407,0.024168588],"study_design_scores_gemma":[0.00005571325,0.00012280744,0.4391519,0.000010007534,0.000090720474,0.00016052266,0.000088949666,0.5447028,0.014643447,0.00041727896,0.00052491494,0.00003086114],"about_ca_topic_score_codex":0.0060011093,"about_ca_topic_score_gemma":0.0065884516,"teacher_disagreement_score":0.0060011093,"about_ca_system_score_codex":0.0004995527,"about_ca_system_score_gemma":0.00016334846,"threshold_uncertainty_score":0.011932373},"labels":[],"label_agreement":null},{"id":"W4390796298","doi":"10.3847/1538-4357/acff64","title":"Stochastic Modeling of Star Formation Histories. III. Constraints from Physically Motivated Gaussian Processes","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Physics; Star formation; Galaxy; Astrophysics; Autocovariance; Spectral density; Galaxy formation and evolution; Statistical physics; Population; Milky Way; Astronomy; Fourier transform; Statistics","score_opus":0.01013745391934608,"score_gpt":0.21223668134606766,"score_spread":0.20209922742672157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390796298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.60595095,0.00034279743,0.38532794,0.0009424152,0.000034714692,0.000049672515,0.00036071948,0.0001726664,0.0068181437],"genre_scores_gemma":[0.99293464,0.00014065363,0.0049658376,0.000065612,0.000030775016,0.000030581894,0.00015347704,0.000026335123,0.0016521856],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99934787,0.00025906277,0.000030206984,0.00012202926,0.00012480997,0.00011596815],"domain_scores_gemma":[0.9944528,0.0035321442,0.0010883978,0.00037448268,0.00036042815,0.00019177205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0023229027,0.0004634625,0.0007246127,0.0005288576,0.00039701854,0.0012676832,0.0011788708,0.0008164218,0.0010984282],"category_scores_gemma":[0.0106745595,0.00047760564,0.00081645214,0.00041886955,0.0014630222,0.001774154,0.00087120046,0.00089771656,0.0001657395],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003328796,0.000025893287,0.0044305567,0.000017047223,0.000029399309,0.0000831055,0.00010318391,0.85447663,0.0010960652,0.13723908,0.00023562428,0.0022301406],"study_design_scores_gemma":[0.0000058286455,0.000008339234,0.0007436018,0.0000022649363,0.0000030033616,0.000009972792,0.000007709038,0.97323644,0.000072237715,0.025756305,0.00014878852,0.0000055103046],"about_ca_topic_score_codex":0.014524232,"about_ca_topic_score_gemma":0.0060538594,"teacher_disagreement_score":0.014524232,"about_ca_system_score_codex":0.0012557134,"about_ca_system_score_gemma":0.0007891257,"threshold_uncertainty_score":0.028879344},"labels":[],"label_agreement":null},{"id":"W4390821164","doi":"10.3847/1538-4357/ad0cbd","title":"Mapping Obscured Star Formation in the Host Galaxy of FRB 20201124A","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Research Corporation for Science Advancement; Ministerio de Ciencia e Innovación; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Agencia Estatal de Investigación; National Radio Astronomy Observatory; Northwestern University; Nuclear Safety and Security Commission; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; David and Lucile Packard Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Magnetar; Jansky; Star formation; Galaxy; Luminosity; Astronomy; Fast radio burst; Radio galaxy; Pulsar","score_opus":0.016721978175139533,"score_gpt":0.3054992526670648,"score_spread":0.28877727449192525,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390821164","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99834013,0.00013282229,0.0002064968,0.000025700398,0.0000055239116,0.0000043360074,0.00037619294,0.000035861456,0.0008728965],"genre_scores_gemma":[0.9977895,0.00005603104,0.00045082983,0.000018296607,0.000014685202,0.0000067046853,0.0012482273,0.000010951691,0.00040493815],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988556,0.0000068853983,0.0000045055535,0.000035618974,0.000027976994,0.000039359104],"domain_scores_gemma":[0.99950767,0.00003210702,0.0001905974,0.000044667413,0.000049939903,0.00017504185],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019544031,0.00033690254,0.0002913145,0.001650421,0.00047541835,0.00058774126,0.0003732759,0.00033787265,0.002377843],"category_scores_gemma":[0.00037072608,0.00019957608,0.00029757095,0.0005615625,0.00019680934,0.00020668638,0.0004084372,0.0002503872,0.0006966906],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040276465,0.00013602625,0.8358211,0.000058450227,0.000118148295,0.0009678025,0.00040017054,0.0006072124,0.14301322,0.00017268985,0.00107876,0.017223693],"study_design_scores_gemma":[0.0000061049086,0.000054045173,0.9969177,0.0000054203197,0.000013419028,0.00029290025,0.0000788304,0.00037481202,0.0011637554,0.000027955815,0.0010600393,0.0000050315693],"about_ca_topic_score_codex":0.005868359,"about_ca_topic_score_gemma":0.009910591,"teacher_disagreement_score":0.005868359,"about_ca_system_score_codex":0.00040126865,"about_ca_system_score_gemma":0.00008860532,"threshold_uncertainty_score":0.011668384},"labels":[],"label_agreement":null},{"id":"W4390825445","doi":"10.3847/1538-4357/ad10ae","title":"Star Formation Efficiency in Nearby Galaxies Revealed with a New CO-to-H<sub>2</sub> Conversion Factor Prescription","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":28,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Royal Society; Science and Technology Facilities Council; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Velocity dispersion; Metallicity; Galaxy formation and evolution; Astronomy","score_opus":0.007962076046158728,"score_gpt":0.21032385378927163,"score_spread":0.2023617777431129,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390825445","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99889636,0.000037011152,0.0005675438,0.00000855149,8.6930885e-7,0.0000033114832,0.0001609001,0.000020517109,0.00030490174],"genre_scores_gemma":[0.99949586,0.000008140784,0.00030637902,0.0000035015514,0.0000012973893,0.0000018667516,0.00014831778,0.0000017515733,0.00003285132],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99981016,0.00003087664,0.00001858726,0.000066091656,0.00004380553,0.000030390987],"domain_scores_gemma":[0.9982522,0.00041216382,0.00074064714,0.0002491857,0.00016360881,0.00018210312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004580078,0.00022897187,0.00020408635,0.0007978989,0.00019730125,0.0006573109,0.00030908594,0.00030833308,0.00048356852],"category_scores_gemma":[0.0013834836,0.00013319768,0.00023994889,0.0006665921,0.00038208606,0.00037355037,0.00036716787,0.00021221452,0.00013879657],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006196926,0.000013063229,0.9918616,0.000006384202,0.000029384446,0.00003185344,0.000034830526,0.0012195561,0.0050211954,0.00008287272,0.000043311138,0.0015939478],"study_design_scores_gemma":[0.0000027418578,0.000021171749,0.993381,0.0000011650005,0.000013221616,0.000048770522,0.000028651468,0.004651382,0.0016914569,0.0000398031,0.00011769663,0.0000029726075],"about_ca_topic_score_codex":0.005515739,"about_ca_topic_score_gemma":0.00742276,"teacher_disagreement_score":0.005515739,"about_ca_system_score_codex":0.00050575874,"about_ca_system_score_gemma":0.00013943277,"threshold_uncertainty_score":0.010967255},"labels":[],"label_agreement":null},{"id":"W4390870627","doi":"10.3847/1538-4357/ad0e68","title":"Ultradeep ATCA Imaging of 47 Tucanae Reveals a Central Compact Radio Source","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; UK Research and Innovation; Nuclear Safety and Security Commission; Federation University Australia; Australian Government; Commonwealth Scientific and Industrial Research Organisation; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Globular cluster; Telescope; Black hole (networking); Astronomy; White dwarf; Compact star; Millisecond pulsar; Radio telescope; Cluster (spacecraft); Intermediate-mass black hole; Pulsar; Galaxy; Stars; Supermassive black hole","score_opus":0.009835273919736195,"score_gpt":0.23408827648446714,"score_spread":0.22425300256473096,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390870627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958198,0.00011903009,0.00019874185,0.000031648993,0.0000049537393,0.000005235501,0.00046284858,0.000035400164,0.0033222237],"genre_scores_gemma":[0.99715817,0.000059212885,0.0005013889,0.000029759036,0.0000086514565,0.000008358876,0.00097405055,0.000009717897,0.001250628],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989104,0.0000026064129,0.0000020781024,0.000020938194,0.000039074745,0.00004427647],"domain_scores_gemma":[0.9997551,0.000015492813,0.000030501795,0.000024424158,0.00009794852,0.00007648774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010258754,0.0001506925,0.00022348412,0.0010915347,0.0010020097,0.0007113276,0.0005448532,0.0003096596,0.0015398485],"category_scores_gemma":[0.00022942203,0.00012218718,0.00014034864,0.0009181494,0.00023099383,0.00014663082,0.0005237949,0.00023023873,0.00027651488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005013697,0.00017964355,0.64984155,0.00007890801,0.00017266186,0.0019625449,0.001568638,0.002309906,0.24477485,0.00066878076,0.005033709,0.09290743],"study_design_scores_gemma":[0.000005816729,0.000021947666,0.9931901,0.00001028945,0.000017702238,0.00019838686,0.00035751547,0.0011189281,0.0021152203,0.00004559126,0.0029112087,0.000007329552],"about_ca_topic_score_codex":0.16869102,"about_ca_topic_score_gemma":0.28352606,"teacher_disagreement_score":0.16869102,"about_ca_system_score_codex":0.000990742,"about_ca_system_score_gemma":0.0005943536,"threshold_uncertainty_score":0.33541828},"labels":[],"label_agreement":null},{"id":"W4390886821","doi":"10.3847/1538-4357/ad0f1b","title":"Simulating the Detection of the Global 21 cm Signal with MIST for Different Models of the Soil and Beam Directivity","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Agencia Nacional de Investigación y Desarrollo","keywords":"Chromaticity; Directivity; Physics; SIGNAL (programming language); Antenna (radio); Optics; Beam (structure); Remote sensing; Acoustics; Telecommunications; Geology; Computer science","score_opus":0.0094419879964244,"score_gpt":0.21586589811747367,"score_spread":0.20642391012104927,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390886821","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99467367,0.00002774895,0.0036970684,0.000094858384,0.000013485315,0.000013622342,0.0004298541,0.00012857284,0.0009211433],"genre_scores_gemma":[0.9979493,0.000015938323,0.0014569586,0.000024152603,0.000003914133,0.000012622701,0.00033449192,0.000016812213,0.0001858432],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997992,0.000054988814,0.000009747939,0.000045301116,0.00003341773,0.000057387457],"domain_scores_gemma":[0.9984274,0.0010005524,0.00014248143,0.00013727628,0.00018864493,0.00010363482],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049700285,0.00051081536,0.0003501731,0.00032426702,0.00038997844,0.00047654787,0.0009862309,0.0011946087,0.0010731877],"category_scores_gemma":[0.002212103,0.0003312584,0.00089938217,0.00066324614,0.00063365605,0.00057131756,0.0003366155,0.0007911718,0.00013382238],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015985468,0.00007781644,0.017144952,0.000020025645,0.000041525058,0.00007554963,0.000049296665,0.97807854,0.0025313958,0.00035969605,0.00020052488,0.0012609167],"study_design_scores_gemma":[0.000064452404,0.00005983136,0.008979252,0.000004368275,0.000021281205,0.000017073122,0.000040015286,0.9889101,0.0015840713,0.00016559433,0.00013550752,0.000018514698],"about_ca_topic_score_codex":0.04832164,"about_ca_topic_score_gemma":0.033308752,"teacher_disagreement_score":0.04832164,"about_ca_system_score_codex":0.0012032407,"about_ca_system_score_gemma":0.00066525297,"threshold_uncertainty_score":0.09608072},"labels":[],"label_agreement":null},{"id":"W4390907531","doi":"10.3847/1538-4357/ad07d1","title":"Search for Galactic Core-collapse Supernovae in a Decade of Data Taken with the IceCube Neutrino Observatory","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; National Research Foundation; Michigan State University; University of Oxford; Chiba University; Santen; Compute Canada; Marquette University","keywords":"Supernova; Physics; Neutrino; Observatory; Stars; Astrophysics; Nuclear physics","score_opus":0.046924687479938124,"score_gpt":0.2879776606997972,"score_spread":0.24105297321985908,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390907531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.84475815,0.0031940648,0.0043991897,0.0024779013,0.00028656764,0.00016246777,0.11886916,0.0013090164,0.024543429],"genre_scores_gemma":[0.8112845,0.0015111142,0.011450199,0.0009537944,0.0002734606,0.00014102156,0.16971165,0.000541515,0.0041327053],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995307,0.00006959485,0.000035309742,0.00013083039,0.00017491805,0.00005870593],"domain_scores_gemma":[0.99769586,0.00038663452,0.00055991363,0.00026243448,0.00066384685,0.00043118952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014884348,0.000359454,0.00040618452,0.0023064788,0.00043400328,0.0012639854,0.00044915828,0.0004669983,0.0023541476],"category_scores_gemma":[0.0031245248,0.00028465388,0.0003568638,0.0027746682,0.00022299627,0.0006183506,0.0009847714,0.0006506432,0.0014525349],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004102665,0.00010534486,0.91622853,0.00014155867,0.0002560321,0.0005475998,0.00030890465,0.0014062279,0.008135488,0.00089967466,0.04349213,0.02806817],"study_design_scores_gemma":[0.00005225868,0.00005875837,0.93398803,0.00013769759,0.00009375226,0.00031719884,0.00038983783,0.0030549334,0.0034001549,0.0006424805,0.057832755,0.000032088385],"about_ca_topic_score_codex":0.02042021,"about_ca_topic_score_gemma":0.045113318,"teacher_disagreement_score":0.02042021,"about_ca_system_score_codex":0.0008360716,"about_ca_system_score_gemma":0.00069653464,"threshold_uncertainty_score":0.040602744},"labels":[],"label_agreement":null},{"id":"W4390907655","doi":"10.3847/1538-4357/ad07e3","title":"JADES: Resolving the Stellar Component and Filamentary Overdense Environment of Hubble Space Telescope (HST)-dark Submillimeter Galaxy HDF850.1 at z = 5.18","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Isaac Newton Trust; Science and Technology Facilities Council; European Commission; European Resuscitation Council; University of Arizona; University of California, Santa Cruz; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Astronomy; James Webb Space Telescope; Star formation; Submillimeter Array; Hubble Deep Field; Luminous infrared galaxy; Galaxy formation and evolution; Hubble space telescope","score_opus":0.008104037631392289,"score_gpt":0.20067083783397285,"score_spread":0.19256680020258057,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390907655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9948154,0.00009697253,0.0013049385,0.00006838556,0.000014752057,0.000010977581,0.001986241,0.00045654483,0.0012458354],"genre_scores_gemma":[0.98794156,0.00007396065,0.006363676,0.00006966465,0.000038217448,0.00001239633,0.0045915204,0.00005608859,0.00085278635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992514,0.000008396921,0.0000036556971,0.000022385511,0.000014884842,0.000025523568],"domain_scores_gemma":[0.99980086,0.0000134257125,0.0000536066,0.000031091942,0.000030826333,0.00007017095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020111632,0.0003262653,0.00021385329,0.0016871972,0.0002873213,0.00057765935,0.00029596614,0.00021611915,0.0016370384],"category_scores_gemma":[0.00028187386,0.00013934745,0.0002612436,0.0005089086,0.00009889513,0.00022222029,0.00032587268,0.0001761509,0.00046892578],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006002931,0.0004424294,0.77115864,0.000096009106,0.00039198453,0.00086556503,0.00059767114,0.00708173,0.12858391,0.0009799217,0.02140529,0.06779665],"study_design_scores_gemma":[0.00003948819,0.000060041766,0.9762506,0.000010514856,0.000044906978,0.00020280937,0.00024204078,0.015073282,0.0045662345,0.00021310624,0.003286808,0.000010260617],"about_ca_topic_score_codex":0.0059089847,"about_ca_topic_score_gemma":0.014297712,"teacher_disagreement_score":0.0059089847,"about_ca_system_score_codex":0.00020798162,"about_ca_system_score_gemma":0.00017726666,"threshold_uncertainty_score":0.011749208},"labels":[],"label_agreement":null},{"id":"W4390907984","doi":"10.3847/1538-4357/acfb83","title":"An Updated Mass–Radius Analysis of the 2017–2018 NICER Data Set of PSR J0030+0451","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":189,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Nuclear Safety and Security Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Centre National d’Etudes Spatiales; Natural Sciences and Engineering Research Council of Canada; European Commission; National Aeronautics and Space Administration","keywords":"Physics; RADIUS; Astrophysics","score_opus":0.032965882619641514,"score_gpt":0.37464754391108857,"score_spread":0.34168166129144706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390907984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9731242,0.0006399886,0.00762918,0.0006010382,0.00007632094,0.000035774592,0.013150236,0.0016589453,0.0030842964],"genre_scores_gemma":[0.95481604,0.00016253648,0.008580662,0.00019734967,0.00018608545,0.000040769668,0.034572635,0.0005805468,0.0008633277],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989503,0.00030188906,0.00007042045,0.00033686063,0.00019910233,0.00014143158],"domain_scores_gemma":[0.9974239,0.000550877,0.0005490091,0.0007787073,0.0004850818,0.00021248664],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024096179,0.0005502976,0.0007057065,0.0030329635,0.0005280225,0.0011699593,0.0010625533,0.0006415109,0.002130049],"category_scores_gemma":[0.004623627,0.00036487833,0.0019662683,0.0014226462,0.0005491878,0.0008681183,0.0014813732,0.00067081675,0.0016883637],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007855946,0.00013242409,0.8518755,0.00035399172,0.0014300233,0.001271159,0.0008586348,0.03934849,0.023655523,0.0028419537,0.030342154,0.047104515],"study_design_scores_gemma":[0.000085720785,0.00008558192,0.8896789,0.00007126252,0.0004625033,0.0006676066,0.0002808126,0.08363504,0.0031781008,0.0012010577,0.02053235,0.00012096503],"about_ca_topic_score_codex":0.021566086,"about_ca_topic_score_gemma":0.022174414,"teacher_disagreement_score":0.021566086,"about_ca_system_score_codex":0.0007115283,"about_ca_system_score_gemma":0.00042296387,"threshold_uncertainty_score":0.04288113},"labels":[],"label_agreement":null},{"id":"W4390908152","doi":"10.3847/1538-4357/ad055c","title":"The Dependence of the Structure of Planet-opened Gaps in Protoplanetary Disks on Radiative Cooling","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Planet; Radiative transfer; Radiative cooling; Thermal; Astrophysics; Protoplanetary disk; Computational physics; Planetary mass; Viscosity; Relaxation (psychology); Angular momentum; Isothermal process; Scale height; Planetary system; Classical mechanics; Optics; Thermodynamics","score_opus":0.00709848412285949,"score_gpt":0.23690818000170497,"score_spread":0.22980969587884548,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390908152","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994165,0.000022118053,0.00015736045,0.000015057232,7.6302155e-7,9.465252e-7,0.00006911988,0.000016433434,0.00030172736],"genre_scores_gemma":[0.99987364,0.000005292297,0.000056905097,0.0000014174791,4.256811e-7,6.737081e-7,0.000036052712,0.0000040467,0.000021418211],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9999552,0.000008802377,0.0000032009634,0.000014270701,0.000004980192,0.000013551309],"domain_scores_gemma":[0.99917394,0.00047141284,0.00015564088,0.00006435358,0.000049544546,0.00008500913],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002297206,0.00017597497,0.00013490114,0.00029578814,0.00016150036,0.00043015237,0.0002582651,0.00025337757,0.0010243166],"category_scores_gemma":[0.0017355665,0.00018597841,0.00020570593,0.00017118001,0.00036434806,0.00035922445,0.00035567096,0.00029605813,0.00009953754],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00079374446,0.00023101574,0.54718626,0.00013965959,0.00015415435,0.00063759,0.00046631516,0.33000833,0.10680264,0.002943999,0.00063876313,0.009997513],"study_design_scores_gemma":[0.00005029541,0.00009489997,0.4738544,0.000016304859,0.000029240518,0.00011533063,0.00013132064,0.5110061,0.013541988,0.00088290597,0.0002540241,0.00002311951],"about_ca_topic_score_codex":0.0022163717,"about_ca_topic_score_gemma":0.0011087476,"teacher_disagreement_score":0.0022163717,"about_ca_system_score_codex":0.00024403543,"about_ca_system_score_gemma":0.0000949034,"threshold_uncertainty_score":0.0044069886},"labels":[],"label_agreement":null},{"id":"W4390941343","doi":"10.3847/1538-4357/ad0893","title":"Proposed Host Galaxies of Repeating Fast Radio Burst Sources Detected by CHIME/FRB","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":40,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of British Columbia; McGill University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"Fonds de recherche du Québec – Nature et technologies; University of Toronto; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Canada Research Chairs; Smithsonian Astrophysical Observatory; National Science Foundation; Ministério da Ciência e Tecnologia; Comisión Nacional de Investigación Científica y Tecnológica; McGill University; Canadian Institute for Advanced Research; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Redshift; Radio galaxy; Population; Peculiar galaxy; Galaxy group","score_opus":0.007039460299688132,"score_gpt":0.27682345659976754,"score_spread":0.26978399630007943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390941343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949315,0.00032424653,0.002291634,0.00009764546,0.0000063190587,0.0000155694,0.0005694423,0.00019752333,0.0015660238],"genre_scores_gemma":[0.99779296,0.00003762326,0.0013919254,0.000030027879,0.000009482415,0.0000058075952,0.000556118,0.000012495535,0.00016345075],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997522,0.000023770775,0.0000092382925,0.000085149724,0.00006204122,0.0000675119],"domain_scores_gemma":[0.99857306,0.00023283191,0.0005682265,0.0001643007,0.0001046659,0.0003569849],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072525453,0.00030074193,0.00044225453,0.0020848073,0.0006016501,0.0010232491,0.0005542477,0.0005272535,0.0024693732],"category_scores_gemma":[0.001098889,0.00028847935,0.00030536987,0.0010760034,0.00046964016,0.0002483113,0.00088052487,0.00032900274,0.00061051844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022234146,0.00003118015,0.96562374,0.00003055244,0.00008694197,0.00044578945,0.00020904723,0.0006975791,0.02165929,0.00073381467,0.0004477103,0.009812149],"study_design_scores_gemma":[0.000019005425,0.000046594017,0.992743,0.00000960401,0.00003464664,0.00064549036,0.0001461594,0.0029443747,0.0017708553,0.0005322369,0.0010913691,0.000016628095],"about_ca_topic_score_codex":0.002308332,"about_ca_topic_score_gemma":0.0027835723,"teacher_disagreement_score":0.9976917,"about_ca_system_score_codex":0.00035552387,"about_ca_system_score_gemma":0.00018906766,"threshold_uncertainty_score":0.008260846},"labels":[],"label_agreement":null},{"id":"W4390945847","doi":"10.3847/1538-4357/ad089a","title":"Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Millisecond pulsar; Globular cluster; Astrophysics; Neutron star; Pulsar; Star cluster; Astronomy; Milky Way; White dwarf; Stars; X-ray pulsar; X-ray binary; Millisecond","score_opus":0.01356496731283635,"score_gpt":0.30908895197027586,"score_spread":0.2955239846574395,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390945847","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982887,0.00006029307,0.0011059509,0.000017295948,0.0000034584175,0.0000026169116,0.000021864544,0.0000097885795,0.00049004296],"genre_scores_gemma":[0.99966264,0.000031222833,0.0001190331,0.00000229167,0.00000183016,0.0000015070315,0.000030034209,0.0000018776069,0.00014951355],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994624,0.0000073047563,0.0000034181408,0.000015115151,0.000011613429,0.000016288526],"domain_scores_gemma":[0.99979013,0.000039813902,0.000072083414,0.000024729172,0.000013481893,0.000059765753],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001847895,0.00027680318,0.0002767929,0.00033969115,0.00044193259,0.00060616346,0.0003161215,0.00029052346,0.0006563575],"category_scores_gemma":[0.0005913393,0.0001595896,0.0003083504,0.00022559846,0.0004703341,0.00045231736,0.00089193246,0.00019960651,0.00009130722],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003496006,0.00016832094,0.49551395,0.00013793183,0.0002449403,0.0015488642,0.0007142429,0.43174714,0.035302136,0.018211769,0.0007134783,0.015347596],"study_design_scores_gemma":[0.00008188527,0.00022595853,0.3102028,0.0000209834,0.00012321919,0.0008840009,0.00056096393,0.6613324,0.006936926,0.018130774,0.0014621308,0.000037987298],"about_ca_topic_score_codex":0.0049138526,"about_ca_topic_score_gemma":0.0032575473,"teacher_disagreement_score":0.0049138526,"about_ca_system_score_codex":0.00053677626,"about_ca_system_score_gemma":0.00033739608,"threshold_uncertainty_score":0.009770513},"labels":[],"label_agreement":null},{"id":"W4390955395","doi":"10.3847/1538-4357/ad0d9f","title":"The Discovery of the Faintest Known Milky Way Satellite Using UNIONS","year":2024,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; University of Toronto; Herzberg Institute of Astrophysics; University of Victoria","funders":"Institut national des sciences de l'Univers; Centre National de la Recherche Scientifique; Canadian Space Agency; Nuclear Safety and Security Commission; National Astronomical Observatory of Japan; NASA Exoplanet Science Institute; National Aeronautics and Space Administration; California Institute of Technology; European Space Agency; W. M. Keck Foundation","keywords":"Physics; Astrophysics; Algorithm; Computer science","score_opus":0.015097071466416404,"score_gpt":0.24020996645450587,"score_spread":0.22511289498808948,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390955395","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9717791,0.0021460007,0.0019461738,0.000539171,0.00007118384,0.000017356184,0.00067728135,0.00039547146,0.022428267],"genre_scores_gemma":[0.99044317,0.0005841287,0.0023992609,0.00028761712,0.000085972926,0.000012252021,0.0013028599,0.000052968047,0.004831787],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99967027,0.000019457191,0.000011150238,0.00014607083,0.00009160208,0.000061352344],"domain_scores_gemma":[0.9993093,0.00010976393,0.00020742751,0.00015576414,0.000070823386,0.00014690503],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004405494,0.00025639043,0.0002781577,0.0012103751,0.0010995572,0.0018315424,0.00060647755,0.00084031106,0.0027635822],"category_scores_gemma":[0.000980132,0.0003331536,0.00032392438,0.0006232196,0.0006487512,0.0008968522,0.0015721761,0.0007199538,0.001195232],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001460081,0.00017252336,0.49929273,0.0005965789,0.0002863779,0.006559793,0.005842324,0.0012812724,0.23755924,0.02748257,0.015637798,0.20382878],"study_design_scores_gemma":[0.00008678711,0.0006096301,0.49177614,0.00029999917,0.00030710702,0.0092948,0.0020832582,0.002851534,0.1148113,0.0065588593,0.3712232,0.00009736692],"about_ca_topic_score_codex":0.0022554658,"about_ca_topic_score_gemma":0.0025238467,"teacher_disagreement_score":0.0027635822,"about_ca_system_score_codex":0.0008378469,"about_ca_system_score_gemma":0.00029567452,"threshold_uncertainty_score":0.009245038},"labels":[],"label_agreement":null},{"id":"W4390987248","doi":"10.3847/1538-4357/ad0b7d","title":"KilonovAE: Exploring Kilonova Spectral Features with Autoencoders","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Kilonova; Physics; Astrophysics; Ejecta; Context (archaeology); Spectral line; Astronomy; Supernova","score_opus":0.017990877067133114,"score_gpt":0.23344048692578415,"score_spread":0.21544960985865103,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390987248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6026606,0.0009871,0.38772938,0.0007054526,0.00017329554,0.00007804669,0.0010029046,0.0043528015,0.0023105678],"genre_scores_gemma":[0.8975288,0.0001547124,0.098273695,0.00022246144,0.00005064536,0.00008036423,0.0021513754,0.00021085862,0.0013270212],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984765,0.000038637354,0.000007705144,0.00004868612,0.000025208263,0.000032064625],"domain_scores_gemma":[0.9991767,0.0005744328,0.0000614686,0.000059599573,0.000090723406,0.00003702277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00071560027,0.0010071934,0.0005934202,0.0007134893,0.0003236669,0.0007640517,0.0012144054,0.0010087914,0.0012608735],"category_scores_gemma":[0.001766221,0.00049975887,0.0009395799,0.0004436213,0.00044045487,0.0008377883,0.0007731764,0.0013835205,0.00030163437],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020526558,0.00019191919,0.0051755556,0.000073436495,0.00015222884,0.0001461334,0.00009300647,0.9193766,0.0045774286,0.002144195,0.002570922,0.0652932],"study_design_scores_gemma":[0.000002416543,0.000006003861,0.00026225654,0.0000026818734,0.0000026944172,0.0000031112443,0.000006868097,0.9988342,0.00024512067,0.0005510759,0.00008116901,0.000002422762],"about_ca_topic_score_codex":0.011987895,"about_ca_topic_score_gemma":0.011901608,"teacher_disagreement_score":0.011987895,"about_ca_system_score_codex":0.0008527673,"about_ca_system_score_gemma":0.00061891036,"threshold_uncertainty_score":0.023836255},"labels":[],"label_agreement":null},{"id":"W4390987280","doi":"10.3847/1538-4357/ad0c4e","title":"A Census of Star Formation Histories of Massive Galaxies at 0.6 &lt; z &lt; 1 from Spectrophotometric Modeling Using Bagpipes and Prospector","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Research Corporation for Scientific Advancement; Pittsburgh Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Stellar mass; Astronomy; Stellar population; Galaxy formation and evolution; Population","score_opus":0.013007348069534791,"score_gpt":0.2185902398294906,"score_spread":0.2055828917599558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390987280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99492526,0.00001885023,0.0022841305,0.000023075667,8.4363813e-7,0.0000055401665,0.002321776,0.00012863897,0.0002918302],"genre_scores_gemma":[0.9892539,0.000024365316,0.0020871768,0.000010823886,0.000004668981,0.000008355417,0.008385384,0.000023348513,0.00020185471],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998336,0.00003920037,0.000006806366,0.00005861204,0.00003500923,0.000026753241],"domain_scores_gemma":[0.99913055,0.00023022344,0.00020239386,0.00017057419,0.00011436453,0.0001520061],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007177007,0.00022566969,0.00023059508,0.0009994411,0.00017809359,0.00046799448,0.0004242207,0.00021060013,0.0007603811],"category_scores_gemma":[0.0017154654,0.00017564355,0.00052179093,0.0008059645,0.00019073221,0.00039835036,0.0006258821,0.0002665935,0.0003548258],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000190061,0.00008737216,0.9274211,0.000023054838,0.00013449545,0.00014652345,0.00027703866,0.044719238,0.004835194,0.0009895877,0.0014745264,0.019701868],"study_design_scores_gemma":[0.000011254167,0.00007428763,0.81451255,0.000006572803,0.000031427808,0.00013409714,0.000104425606,0.1811625,0.0016982293,0.0006715973,0.0015722523,0.000020725396],"about_ca_topic_score_codex":0.00975662,"about_ca_topic_score_gemma":0.007963664,"teacher_disagreement_score":0.00975662,"about_ca_system_score_codex":0.00032447916,"about_ca_system_score_gemma":0.00019113456,"threshold_uncertainty_score":0.019399643},"labels":[],"label_agreement":null},{"id":"W4390987285","doi":"10.3847/1538-4357/ad0cc1","title":"Magnetic Fields of the Starless Core L 1512","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Canadian Space Agency; National Science and Technology Council; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; National Astronomical Observatory of Japan; National Tsing Hua University; Centre National de la Recherche Scientifique; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Jet Propulsion Laboratory; Centre National d’Etudes Spatiales; Ministry of Science and Technology, Taiwan; California Institute of Technology; Academia Sinica; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Astronomical Research Institute of Thailand; W. M. Keck Foundation; National Science Foundation","keywords":"Physics; Magnetic field; Astrophysics; Faraday effect; Polarization (electrochemistry); Field strength; Molecular cloud; Astronomy; Stars","score_opus":0.01230208785461917,"score_gpt":0.2426703240736692,"score_spread":0.23036823621905003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390987285","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984125,0.000039616578,0.000058775295,0.000017995542,0.0000024831775,0.0000031666686,0.00013556615,0.000015308198,0.0013145979],"genre_scores_gemma":[0.99929655,0.000010636292,0.00007756194,0.00002312402,0.0000044123703,0.00000201132,0.0003859754,0.0000049051473,0.0001948892],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999231,0.0000044428452,0.0000037991447,0.000027533542,0.000022835733,0.000018192746],"domain_scores_gemma":[0.9998253,0.000009010465,0.000039072173,0.000014468925,0.000025575133,0.000086585766],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000102593214,0.00026060775,0.0003119519,0.00055695936,0.0003997912,0.00047794337,0.00038332338,0.00030542142,0.00090514595],"category_scores_gemma":[0.00022376556,0.0001419397,0.00014718666,0.00027801876,0.00029309856,0.00020875946,0.0007209699,0.00024505408,0.00034804223],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000558131,0.00015850746,0.6067386,0.000069621776,0.00010235574,0.0024605223,0.0010248306,0.0010239074,0.37638444,0.0004662654,0.0011730383,0.009839834],"study_design_scores_gemma":[0.000019195888,0.00007850523,0.992176,0.0000059370886,0.000015061896,0.0004491331,0.00020064494,0.0012353016,0.0045614066,0.00005107551,0.0011971012,0.000010702343],"about_ca_topic_score_codex":0.0048814663,"about_ca_topic_score_gemma":0.0053436183,"teacher_disagreement_score":0.0048814663,"about_ca_system_score_codex":0.00047128444,"about_ca_system_score_gemma":0.00015693417,"threshold_uncertainty_score":0.00970614},"labels":[],"label_agreement":null},{"id":"W4390987761","doi":"10.3847/1538-4357/ad1400","title":"The CO Outflow Components Ejected by a Recent Accretion Event in B335","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea","keywords":"Physics; Astrophysics; Accretion (finance); Outflow; Protostar; Astronomy; Brightness; Millimeter; Submillimeter Array; Accretion disc; Stars; Star formation","score_opus":0.011626587818012213,"score_gpt":0.265681882777454,"score_spread":0.2540552949594418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390987761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997552,0.00003879239,0.00006037151,0.000002977811,8.5223655e-7,8.852305e-7,0.000048109185,0.0000026286457,0.00009027418],"genre_scores_gemma":[0.999739,0.00001324414,0.000048508344,0.000003064132,0.0000014115783,5.101858e-7,0.0001369035,0.000001041463,0.00005629895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996316,0.0000031515067,0.0000032049081,0.000009348289,0.000007878673,0.000013279162],"domain_scores_gemma":[0.9998584,0.000016486249,0.00006762907,0.0000058184964,0.000013132457,0.000038662027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008213905,0.00015264472,0.00012024055,0.0005309524,0.00020737849,0.00027555722,0.00010141966,0.00017974876,0.000718537],"category_scores_gemma":[0.00021299881,0.00007527713,0.00016639348,0.00035282018,0.00011141358,0.000114992574,0.00021219227,0.00010703362,0.000115585564],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026426616,0.00003718576,0.9676395,0.000018011962,0.000034926594,0.0011412897,0.00008438645,0.00042304167,0.025718817,0.000056868743,0.0000809675,0.004500653],"study_design_scores_gemma":[0.000001412449,0.0000125039005,0.99891615,0.0000016644939,0.0000050909475,0.00015433933,0.000027029322,0.00046038145,0.00034662674,0.000007579632,0.000066132576,0.0000011466201],"about_ca_topic_score_codex":0.006952998,"about_ca_topic_score_gemma":0.008010141,"teacher_disagreement_score":0.006952998,"about_ca_system_score_codex":0.00020709373,"about_ca_system_score_gemma":0.00008087774,"threshold_uncertainty_score":0.013825059},"labels":[],"label_agreement":null},{"id":"W4390988088","doi":"10.3847/1538-4357/ad0b77","title":"Brightest Cluster Galaxy Formation in the z = 4.3 Protocluster SPT 2349-56: Discovery of a Radio-loud Active Galactic Nucleus","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Comisión Nacional de Investigación Científica y Tecnológica; Natural Sciences and Engineering Research Council of Canada; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; Max-Planck-Gesellschaft; National Research Foundation; Australian Government; Commonwealth Scientific and Industrial Research Organisation; National Radio Astronomy Observatory; Science and Industry Endowment Fund; Government of Western Australia; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Active galactic nucleus; Astrophysics; Galaxy; Astronomy; Radio galaxy; Submillimeter Array; Radio telescope; Galaxy cluster; Redshift; Luminosity; Luminous infrared galaxy; Star formation; Cluster (spacecraft)","score_opus":0.007668123280063142,"score_gpt":0.22457139262711198,"score_spread":0.21690326934704884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390988088","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990392,0.000048061574,0.00009174414,0.000020628666,0.00000509038,0.0000046765617,0.00011510794,0.000012555222,0.0006630157],"genre_scores_gemma":[0.9991536,0.000024236444,0.00021119142,0.000023410212,0.0000058287183,0.0000029427754,0.00022135963,0.0000048325232,0.00035256403],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998939,0.0000046787864,0.000004491802,0.000033332857,0.000032221586,0.00003134015],"domain_scores_gemma":[0.99974066,0.000011580542,0.00009168825,0.000018845898,0.000037867314,0.00009941765],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099018085,0.00026837637,0.00030849184,0.0007754069,0.0007485642,0.00051603024,0.00048794592,0.00029136532,0.0017538412],"category_scores_gemma":[0.00023344993,0.00016940413,0.00021782794,0.00038310565,0.00047532434,0.00015953497,0.0006890088,0.00027709574,0.0006157899],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024251267,0.000050809136,0.8891688,0.000029052948,0.000058689806,0.0019646992,0.00050473365,0.00015243504,0.10091702,0.00013305972,0.00037580015,0.0064024627],"study_design_scores_gemma":[0.0000038705807,0.00007991822,0.99526274,0.000004266109,0.000015061251,0.0011720462,0.00018566204,0.0001326625,0.0022523007,0.00004372626,0.0008428406,0.000004931196],"about_ca_topic_score_codex":0.006425408,"about_ca_topic_score_gemma":0.008148542,"teacher_disagreement_score":0.006425408,"about_ca_system_score_codex":0.0003899377,"about_ca_system_score_gemma":0.00016251001,"threshold_uncertainty_score":0.012776017},"labels":[],"label_agreement":null},{"id":"W4390988145","doi":"10.3847/1538-4357/ad11d6","title":"Investigating Extreme Scattering Events by Volumetric Ray-tracing","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Ray tracing (physics); Eikonal equation; Paraxial approximation; Scattering; Optics; Computational physics","score_opus":0.015401209179691172,"score_gpt":0.2318582126357712,"score_spread":0.21645700345608002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390988145","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6762435,0.00017323869,0.31433988,0.00019464306,0.00004259339,0.00011987883,0.00022355128,0.00089112937,0.0077715493],"genre_scores_gemma":[0.9604895,0.00006226172,0.038588785,0.000018689389,0.000007914899,0.00001815734,0.0001101219,0.000054427594,0.0006501169],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979407,0.00005378613,0.000009718445,0.00002289982,0.00008447507,0.000035003373],"domain_scores_gemma":[0.9984034,0.0009313288,0.00026150618,0.00011596069,0.00020000509,0.00008794524],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005247586,0.00058135286,0.0003729396,0.00096410984,0.00030669302,0.00091452524,0.0010644464,0.00083152385,0.0012950018],"category_scores_gemma":[0.003257103,0.00023653284,0.00037786405,0.0006115192,0.00063632615,0.0006351577,0.0007160314,0.00048513504,0.00014417377],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005621483,0.00006662168,0.004771458,0.00003236006,0.000020303434,0.00014855422,0.0001304638,0.976542,0.0046063396,0.007560812,0.00017826675,0.00588651],"study_design_scores_gemma":[0.0000033636309,0.000010752179,0.0002037332,0.0000028005034,0.0000010612373,0.000017353228,0.000017855431,0.99837434,0.0006189969,0.0006329944,0.00011319644,0.0000035253472],"about_ca_topic_score_codex":0.00719233,"about_ca_topic_score_gemma":0.0041254824,"teacher_disagreement_score":0.00719233,"about_ca_system_score_codex":0.0007833279,"about_ca_system_score_gemma":0.00048537643,"threshold_uncertainty_score":0.014300942},"labels":[],"label_agreement":null},{"id":"W4390988219","doi":"10.3847/1538-4357/ad09e2","title":"ALMA Survey of Orion Planck Galactic Cold Clumps (ALMASOP): Discovery of an Extremely Dense and Compact Object Embedded in the Prestellar Core G208.68-19.92-N2","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Submillimeter Array; Nucleus; Molecular cloud; RADIUS; Outflow; Millimeter; Virial theorem; Bipolar outflow; Luminosity; Star formation; Stars; Astronomy; Galaxy","score_opus":0.03187812448496121,"score_gpt":0.28508031131266776,"score_spread":0.25320218682770657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4390988219","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988643,0.00008594322,0.00004390032,0.000020631112,0.0000022772936,0.0000058964038,0.00035555105,0.000013354116,0.000608159],"genre_scores_gemma":[0.99811494,0.00006516391,0.00022937894,0.000035457768,0.00000971264,0.0000088938,0.0010406389,0.000006699169,0.0004890105],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999007,0.0000063563934,0.000004186226,0.000029236007,0.000029230767,0.000030363955],"domain_scores_gemma":[0.9998234,0.000010093726,0.000047966183,0.000014528921,0.000024990406,0.00007905399],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001485052,0.00024049262,0.00020985788,0.0010561318,0.00048297193,0.0002903623,0.0003066518,0.000255953,0.00075374957],"category_scores_gemma":[0.0001395586,0.00011116801,0.00014885423,0.00047290605,0.00014814752,0.00013128067,0.00049385725,0.00015950699,0.00031129352],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011934456,0.00006263016,0.94934446,0.000033326894,0.000052421816,0.0009537269,0.00045409118,0.00007075141,0.042041022,0.00007991673,0.00073622994,0.0060521625],"study_design_scores_gemma":[0.00000390338,0.00001798837,0.9981079,0.0000028935292,0.000008096018,0.00018340843,0.00013832701,0.00012871454,0.0005267155,0.000010795118,0.00086909055,0.0000020441885],"about_ca_topic_score_codex":0.01013518,"about_ca_topic_score_gemma":0.014626229,"teacher_disagreement_score":0.01013518,"about_ca_system_score_codex":0.00030572497,"about_ca_system_score_gemma":0.00016741137,"threshold_uncertainty_score":0.02015239},"labels":[],"label_agreement":null},{"id":"W4391036677","doi":"10.3847/1538-4357/ad0cea","title":"The Sloan Digital Sky Survey Reverberation Mapping Project: Investigation of Continuum Lag Dependence on Broad-line Contamination and Quasar Properties","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; National Astronomical Observatories, Chinese Academy of Sciences; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Agencia Nacional de Investigación y Desarrollo; Brookhaven National Laboratory; Ministério da Ciência, Tecnologia e Inovação; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; College of Engineering, Michigan State University; Princeton University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Harvard University; Ohio State University; U.S. Department of Energy; Smithsonian Institution; National Science Foundation; New Mexico State University; University of Portsmouth; Institut national des sciences de l'Univers; Vanderbilt University; Yale University","keywords":"Physics; Quasar; Astrophysics; Reverberation mapping; Balmer series; Redshift; Sky; Active galactic nucleus; Emission spectrum; Astronomy; Galaxy; Spectral line; Accretion (finance)","score_opus":0.02049660065614309,"score_gpt":0.22532504065625245,"score_spread":0.20482844000010936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391036677","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986999,0.000021310925,0.00008970353,0.000010578185,6.4036846e-7,0.0000032180149,0.0008998495,0.0000059633458,0.0002688806],"genre_scores_gemma":[0.99633634,0.000022565402,0.00015823981,0.0000075433263,0.0000030864271,0.00000698783,0.0032685183,0.000006206694,0.00019046744],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992718,0.00021255674,0.00005714382,0.00012883627,0.00021313281,0.00011646781],"domain_scores_gemma":[0.9929618,0.0016560997,0.0030026152,0.00079205935,0.0008463593,0.0007411312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014894061,0.00022759996,0.00020983708,0.00178192,0.0003325095,0.0006955121,0.00037708733,0.00019189768,0.0011276798],"category_scores_gemma":[0.0035058816,0.00013286382,0.00023713305,0.001612807,0.00028744817,0.00043126117,0.0006577207,0.00022886142,0.00043298857],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000036516863,0.000018960733,0.9983039,0.0000036336862,0.000022976688,0.000027145416,0.000081539336,0.000068691304,0.00022253582,0.000014883684,0.000110419765,0.0010887568],"study_design_scores_gemma":[9.412301e-7,0.000011358194,0.9995819,6.69001e-7,0.000003219739,0.000025625564,0.000059860016,0.00013729955,0.00007299446,0.0000032156452,0.000102194506,8.150283e-7],"about_ca_topic_score_codex":0.014302745,"about_ca_topic_score_gemma":0.018557308,"teacher_disagreement_score":0.014302745,"about_ca_system_score_codex":0.0002450235,"about_ca_system_score_gemma":0.0002495921,"threshold_uncertainty_score":0.028438985},"labels":[],"label_agreement":null},{"id":"W4391046605","doi":"10.3847/1538-4357/ad1bc6","title":"Testing CCC+TL Cosmology with Observed Baryon Acoustic Oscillation Features","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Ottawa","funders":"","keywords":"Physics; Cosmic microwave background; Baryon acoustic oscillations; Astrophysics; Cosmology; Big Bang nucleosynthesis; Baryon; Galaxy; Nucleosynthesis; Supernova; Universe; Horizon; Spectral density; Astronomy; Dark energy; Anisotropy; Quantum mechanics","score_opus":0.016101939971276163,"score_gpt":0.2468478222713328,"score_spread":0.23074588230005666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391046605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9792809,0.000045581928,0.016394159,0.00015011264,0.00002038832,0.000019626263,0.00022004313,0.00011314509,0.0037559164],"genre_scores_gemma":[0.99805474,0.000010896037,0.0015246567,0.000016224258,0.0000065994777,0.000008463131,0.00014478131,0.000016362848,0.00021726292],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991623,0.00033693964,0.000043060114,0.00021990175,0.00015344341,0.00008433566],"domain_scores_gemma":[0.9959644,0.0014716275,0.0008489716,0.0007558561,0.0005722716,0.00038678816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025722026,0.0006066201,0.00039006802,0.0006439252,0.00034175706,0.0014928635,0.0013390376,0.00051518244,0.0034152255],"category_scores_gemma":[0.0054828874,0.0002717812,0.00073020515,0.00047388254,0.00074203743,0.0009509936,0.0010520683,0.0005222221,0.00041043301],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013493624,0.0004430613,0.6436019,0.00013905352,0.0005404767,0.0004898466,0.0006048868,0.2697611,0.0130308485,0.045333188,0.0016483946,0.023057878],"study_design_scores_gemma":[0.0001431011,0.00037208977,0.099552736,0.00001921317,0.000092429684,0.0002347723,0.00028849384,0.8842983,0.0025537687,0.010768474,0.001624386,0.000052243595],"about_ca_topic_score_codex":0.014614613,"about_ca_topic_score_gemma":0.00669665,"teacher_disagreement_score":0.014614613,"about_ca_system_score_codex":0.0017923844,"about_ca_system_score_gemma":0.00078532303,"threshold_uncertainty_score":0.029059112},"labels":[],"label_agreement":null},{"id":"W4391112744","doi":"10.3847/1538-4357/ad08bf","title":"Exploring the Chemistry and Mass Function of the Globular Cluster 47 Tucanae with New Theoretical Color–Magnitude Diagrams","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Stars; Photometry (optics); Star cluster; Low Mass; Astronomy; Initial mass function; Stellar mass; Cluster (spacecraft); Magnitude (astronomy); Star formation","score_opus":0.011408393340108373,"score_gpt":0.197543842304523,"score_spread":0.1861354489644146,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391112744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9889742,0.00007720957,0.007491306,0.000076159995,0.0000025361494,0.00000830347,0.00021988395,0.00007699787,0.003073388],"genre_scores_gemma":[0.99731904,0.000029907269,0.0020506692,0.000007363856,0.0000020995456,0.000006717822,0.00023442997,0.000009912592,0.0003398769],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995553,0.000006486125,0.0000011241438,0.000012649936,0.0000097863895,0.000014445109],"domain_scores_gemma":[0.99976796,0.00007716042,0.000030082952,0.000019790881,0.00006403177,0.000041074236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021071905,0.0002658792,0.00017877329,0.0012501446,0.0006299978,0.0007968825,0.00066967175,0.0004248261,0.001874098],"category_scores_gemma":[0.0007448526,0.000098801065,0.0002581201,0.0005848511,0.0004391726,0.0003752078,0.00037156904,0.0001869438,0.0001511693],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013680973,0.0000748751,0.2241153,0.000050132367,0.0000745423,0.0002765183,0.00028107484,0.70942813,0.015191837,0.031002542,0.0010882233,0.018280039],"study_design_scores_gemma":[0.000010494845,0.000018081315,0.061823368,0.0000055518813,0.00001571813,0.000035993606,0.00013479253,0.9304239,0.0019979835,0.004201683,0.0013181347,0.000014283023],"about_ca_topic_score_codex":0.08546099,"about_ca_topic_score_gemma":0.037437398,"teacher_disagreement_score":0.08546099,"about_ca_system_score_codex":0.00236355,"about_ca_system_score_gemma":0.00067901507,"threshold_uncertainty_score":0.16992712},"labels":[],"label_agreement":null},{"id":"W4391131929","doi":"10.3847/1538-4357/ad1103","title":"Testing He ii Emission from Wolf–Rayet Stars as a Dust Attenuation Measure in Eight Nearby Star-forming Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Universidad Nacional Autónoma de México; Space Telescope Science Institute; European Southern Observatory; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration","keywords":"Physics; Wolf–Rayet star; Astrophysics; Galaxy; Astronomy; Stars; Extinction (optical mineralogy)","score_opus":0.013775674912010401,"score_gpt":0.22635556024717693,"score_spread":0.21257988533516653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391131929","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99978656,0.000014529259,0.000061293045,0.0000019754505,6.6053803e-7,0.0000035452026,0.000026908192,0.0000038274006,0.000100711666],"genre_scores_gemma":[0.9997247,0.0000054646566,0.00013911286,0.000002964516,0.0000015059454,0.0000027619521,0.000068790236,0.0000010351496,0.000053648233],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995314,0.00008780394,0.000045220793,0.00015565737,0.0000902872,0.00008953385],"domain_scores_gemma":[0.9982576,0.0003578257,0.00040033818,0.00020790713,0.00026927257,0.00050703477],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089670735,0.0003955239,0.0003656015,0.0016857145,0.00062904385,0.00069533713,0.00048627023,0.0004798524,0.0009572214],"category_scores_gemma":[0.0012303425,0.00023099977,0.00027111662,0.0007214404,0.00054889347,0.00040278689,0.00067011104,0.0002596071,0.0003061415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012668315,0.00008545659,0.99008673,0.0000065163617,0.000026153844,0.00006877103,0.0002563682,0.000117442105,0.007589046,0.000016537268,0.000020728537,0.0015994997],"study_design_scores_gemma":[0.0000068036784,0.00018816156,0.99816054,0.0000011801707,0.00001022161,0.0000603314,0.00017838989,0.00028243405,0.0010210031,0.000011941044,0.00007712877,0.000001930207],"about_ca_topic_score_codex":0.0055786795,"about_ca_topic_score_gemma":0.006105526,"teacher_disagreement_score":0.0055786795,"about_ca_system_score_codex":0.0004874683,"about_ca_system_score_gemma":0.00012300443,"threshold_uncertainty_score":0},"labels":[],"label_agreement":null},{"id":"W4391135343","doi":"10.3847/1538-4357/ad0f97","title":"Constraining Neutrino Cosmologies with Nonlinear Reconstruction","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China","keywords":"Physics; Neutrino; Astronomy; Astrophysics; Nonlinear system; Nuclear physics","score_opus":0.00977176325778025,"score_gpt":0.24694495243243833,"score_spread":0.23717318917465807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391135343","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.78747785,0.00017919106,0.20181936,0.00070846436,0.000026525704,0.000027397777,0.00034275374,0.00043832287,0.008980007],"genre_scores_gemma":[0.9747922,0.00007069364,0.024063991,0.00006558195,0.000016096781,0.000010000221,0.00021193284,0.00006320967,0.0007062811],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999795,0.00011011334,0.0000068862264,0.000030499812,0.00003450677,0.000022967379],"domain_scores_gemma":[0.9983541,0.00096091453,0.00021557862,0.00023924132,0.00013916401,0.00009114699],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010553754,0.0005218407,0.00036439547,0.0005302433,0.00030126135,0.0009501205,0.00050546305,0.00040988208,0.0019088427],"category_scores_gemma":[0.005209768,0.000373794,0.00038714806,0.00040369373,0.001229729,0.0012420329,0.001415037,0.00067755516,0.00021327338],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059851346,0.00009918347,0.038443696,0.00014931761,0.00021151733,0.00018971217,0.00021182378,0.8157071,0.021816641,0.089202836,0.0010171464,0.032352474],"study_design_scores_gemma":[0.00002122068,0.000013205393,0.0017450738,0.0000058132136,0.000008177277,0.000013127455,0.000014474118,0.9805386,0.0020400141,0.015362116,0.00022529178,0.000012728567],"about_ca_topic_score_codex":0.0064373,"about_ca_topic_score_gemma":0.005855912,"teacher_disagreement_score":0.0064373,"about_ca_system_score_codex":0.0005669041,"about_ca_system_score_gemma":0.00056920515,"threshold_uncertainty_score":0.01279968},"labels":[],"label_agreement":null},{"id":"W4391168187","doi":"10.3847/1538-4357/ad0c59","title":"Statistical Association between the Candidate Repeating FRB 20200320A and a Galaxy Group","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; University of British Columbia, Okanagan Campus; Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute; York University; University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Redshift; Astrophysics; Galaxy; Halo; Astronomy","score_opus":0.005786933441761085,"score_gpt":0.22224610255365548,"score_spread":0.2164591691118944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391168187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973436,0.000061168816,0.00051090133,0.00005577675,0.0000047297603,0.0000037645448,0.0008823847,0.00006696338,0.0010706286],"genre_scores_gemma":[0.9984915,0.000009563588,0.0001752208,0.000020534471,0.000008719114,0.0000030262995,0.0010586337,0.000012425423,0.0002202833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999514,0.00008762558,0.00002381573,0.0001751246,0.00012253437,0.00007695888],"domain_scores_gemma":[0.9956173,0.001458966,0.00123677,0.0005150827,0.00039721432,0.0007747816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008872206,0.00020366121,0.00028432382,0.001486786,0.0003102811,0.0005706058,0.00030457004,0.0003116781,0.00549765],"category_scores_gemma":[0.0036104154,0.00010383025,0.00036685175,0.0009873318,0.00036304787,0.00022061434,0.0005229979,0.0002985701,0.0008660062],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000752356,0.000010349193,0.99488187,0.000005131172,0.000089736175,0.000056010682,0.00002799569,0.00021510439,0.0016697034,0.00008761674,0.0004725365,0.0024086796],"study_design_scores_gemma":[0.0000032073394,0.000021571093,0.99821305,0.000001710612,0.000019072368,0.00009654963,0.000038392413,0.0009503251,0.00033573754,0.00007141005,0.00024566395,0.0000033178064],"about_ca_topic_score_codex":0.005334507,"about_ca_topic_score_gemma":0.0049757427,"teacher_disagreement_score":0.00549765,"about_ca_system_score_codex":0.00020715437,"about_ca_system_score_gemma":0.00011472839,"threshold_uncertainty_score":0.01839149},"labels":[],"label_agreement":null},{"id":"W4391170291","doi":"10.3847/1538-4357/ad0fe8","title":"Discovery of a Young, Highly Scattered Pulsar PSR J1032-5804 with the Australian Square Kilometre Array Pathfinder","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Australian Research Council; National Science Foundation","keywords":"Pathfinder; Physics; Kilometer; Pulsar; Astronomy; Square (algebra); Astrophysics","score_opus":0.012136531036662594,"score_gpt":0.2945921130946711,"score_spread":0.2824555820580085,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391170291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99817073,0.00006568243,0.000601744,0.000103438164,0.000007332217,0.000010310385,0.000063281936,0.000021344755,0.0009561054],"genre_scores_gemma":[0.99853194,0.0000317705,0.0009525181,0.000061406914,0.0000082006845,0.000006294019,0.00009050263,0.0000038697417,0.00031352264],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977463,0.00002197667,0.000013975164,0.000058195765,0.000096182484,0.00003503031],"domain_scores_gemma":[0.99935406,0.00007671906,0.00020552905,0.00008253232,0.00009464987,0.00018659084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039277383,0.00015128957,0.00025328094,0.0009769342,0.0007568914,0.00060951,0.00038469143,0.000511312,0.0007787618],"category_scores_gemma":[0.00081319915,0.0002529151,0.00021406627,0.0007158035,0.00036075353,0.00030729096,0.00087305903,0.0004834445,0.00033863558],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002159683,0.0001646897,0.82510066,0.00005653289,0.000093355535,0.009178339,0.0017843463,0.0003295021,0.12344495,0.000773517,0.0010667196,0.037791386],"study_design_scores_gemma":[0.000010040006,0.0001056538,0.9927246,0.000005894014,0.000015501375,0.0028531656,0.00014417218,0.00074540445,0.0015419485,0.00018342474,0.0016632054,0.000007145959],"about_ca_topic_score_codex":0.002942579,"about_ca_topic_score_gemma":0.004423642,"teacher_disagreement_score":0.002942579,"about_ca_system_score_codex":0.00026536916,"about_ca_system_score_gemma":0.00020678474,"threshold_uncertainty_score":0.005850911},"labels":[],"label_agreement":null},{"id":"W4391174763","doi":"10.3847/1538-4357/ad1034","title":"The JWST Discovery of the Triply Imaged Type Ia “Supernova H0pe” and Observations of the Galaxy Cluster PLCK G165.7+67.0","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":63,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Astrophysics Science Division; Science and Technology Facilities Council; Goddard Space Flight Center; College of Science, University of Arizona; NASA Headquarters; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Brightest cluster galaxy; Interacting galaxy; Type-cD galaxy; Supernova; Gravitational lens; Galaxy cluster; Galaxy group; Star formation; Dwarf galaxy; Redshift","score_opus":0.010367824913640258,"score_gpt":0.2218831948273526,"score_spread":0.21151536991371234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391174763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99758506,0.00011336386,0.0003870979,0.00008436821,0.000023012099,0.0000094207935,0.00019486256,0.000036912825,0.0015658289],"genre_scores_gemma":[0.9991136,0.00003383106,0.00032304478,0.000039723607,0.000022255888,0.0000017371933,0.00017568933,0.0000049810615,0.00028512],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987245,0.000008248615,0.000008158412,0.000035040586,0.000051906933,0.000024235429],"domain_scores_gemma":[0.99951005,0.000035794965,0.00012125633,0.000040471215,0.000066907094,0.00022542181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030366945,0.00021290075,0.00014977028,0.00078769337,0.0004905861,0.0005563871,0.00026393923,0.00027943464,0.0012828924],"category_scores_gemma":[0.0004619184,0.00021925152,0.0001672917,0.00021806131,0.0004324418,0.00029310863,0.0005730213,0.00034989178,0.00028660204],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004304,0.00012841291,0.8832571,0.00006488265,0.00015311986,0.012579679,0.0004959584,0.00028017428,0.07989198,0.0008336836,0.00297008,0.018914547],"study_design_scores_gemma":[0.000009461417,0.00015107103,0.9864622,0.000009151598,0.00003950398,0.0056644534,0.00017127505,0.00041889603,0.0039601494,0.00014420124,0.0029605718,0.0000091272805],"about_ca_topic_score_codex":0.0042562983,"about_ca_topic_score_gemma":0.006592835,"teacher_disagreement_score":0.0042562983,"about_ca_system_score_codex":0.0004329797,"about_ca_system_score_gemma":0.00014085823,"threshold_uncertainty_score":0.008463085},"labels":[],"label_agreement":null},{"id":"W4391229769","doi":"10.3847/1538-4357/ad072d","title":"An Updated Modular Set of Synthetic Spectral Energy Distributions for Young Stellar Objects","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Nortel (Canada)","funders":"National Science Foundation","keywords":"Physics; Young stellar object; Modular design; Astrophysics; Set (abstract data type); Astronomy; Stellar atmosphere; Energy (signal processing); Spectral energy distribution; Stars; Spectral line; Star formation","score_opus":0.008584738573999405,"score_gpt":0.24628435641711613,"score_spread":0.23769961784311672,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391229769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6255354,0.0002453702,0.23535904,0.0005938693,0.00030385857,0.0003345675,0.08133403,0.04385249,0.012441346],"genre_scores_gemma":[0.718755,0.00018358284,0.1407371,0.0002838464,0.00008052137,0.00045108926,0.13002755,0.0053836824,0.0040975926],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997811,0.000034366876,0.000012269944,0.00006833907,0.000074466516,0.000029490513],"domain_scores_gemma":[0.9991128,0.0001709069,0.000053390482,0.00029565033,0.00028091605,0.000086377055],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008251415,0.00075622706,0.00040515547,0.0008672986,0.0003410464,0.00093621947,0.0013829607,0.0006499639,0.0040152767],"category_scores_gemma":[0.0027236962,0.0004338591,0.0013259117,0.00071438844,0.00021843567,0.0009805486,0.0006997869,0.0007107411,0.003277363],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055882736,0.00048814382,0.14392628,0.0002444212,0.00043728392,0.0004227479,0.00052168476,0.6775617,0.01763322,0.0066433153,0.053439472,0.09812298],"study_design_scores_gemma":[0.00006648679,0.000051108134,0.02096477,0.000020301319,0.000036345624,0.00014429625,0.000054367036,0.94765383,0.0069643687,0.0038038162,0.020175977,0.000064344546],"about_ca_topic_score_codex":0.009978952,"about_ca_topic_score_gemma":0.010322194,"teacher_disagreement_score":0.009978952,"about_ca_system_score_codex":0.00077941135,"about_ca_system_score_gemma":0.00049720827,"threshold_uncertainty_score":0.01984173},"labels":[],"label_agreement":null},{"id":"W4391230929","doi":"10.3847/1538-4357/ad0b7b","title":"JWST MIRI/Medium Resolution Spectrograph (MRS) Observations and Spectral Models of the Underluminous Type Ia Supernova 2022xkq","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"National Aeronautics and Space Administration; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Spectrograph; Supernova; Astronomy; Spectral resolution; Astrophysics; Resolution (logic); Spectral line","score_opus":0.02505817712516894,"score_gpt":0.24566619371975354,"score_spread":0.2206080165945846,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391230929","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99563664,0.00008448922,0.0019343843,0.000041997224,0.000004151085,0.0000077443765,0.00042514104,0.00016658261,0.0016989594],"genre_scores_gemma":[0.99849665,0.00002396085,0.0005896837,0.000014514819,0.0000031084967,0.000005277393,0.00060711184,0.000021970964,0.0002377449],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999521,0.000005547127,0.0000026747875,0.000012978694,0.000012108485,0.000014556631],"domain_scores_gemma":[0.99987936,0.000011205672,0.00004041754,0.000014866299,0.000016230484,0.000037984588],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018999765,0.00037807034,0.00024345813,0.00043953318,0.00021159585,0.0004887296,0.00036744642,0.00026556736,0.0009840769],"category_scores_gemma":[0.0002939731,0.00024482174,0.0004784942,0.00024209039,0.00014954167,0.00025991097,0.00031853752,0.00021566403,0.00028669904],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009195414,0.0001951383,0.6712034,0.00012033432,0.00027798707,0.0018630591,0.00031919542,0.118375145,0.18766814,0.004413418,0.002591253,0.012053359],"study_design_scores_gemma":[0.000048583355,0.00016394883,0.77263886,0.000014387932,0.00006451379,0.00042544072,0.00014526196,0.21522596,0.007716811,0.001339286,0.0021831729,0.000033832202],"about_ca_topic_score_codex":0.0035057017,"about_ca_topic_score_gemma":0.0033003746,"teacher_disagreement_score":0.0035057017,"about_ca_system_score_codex":0.00052137556,"about_ca_system_score_gemma":0.000108575274,"threshold_uncertainty_score":0.0069705844},"labels":[],"label_agreement":null},{"id":"W4391257246","doi":"10.3847/1538-4357/ad0ce8","title":"The Aemulus Project. VI. Emulation of Beyond-standard Galaxy Clustering Statistics to Improve Cosmological Constraints","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"National Energy Research Scientific Computing Center; Directorate for Mathematical and Physical Sciences; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Physics; Galaxy; Redshift; Astrophysics; Statistics; Correlation function (quantum field theory); Halo; Cosmology; Statistical physics; Quantum mechanics","score_opus":0.009813773548352368,"score_gpt":0.2534841991128093,"score_spread":0.24367042556445692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391257246","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6343382,0.00045107107,0.29535744,0.0010593996,0.0002603858,0.00027901,0.012656442,0.03784491,0.017753238],"genre_scores_gemma":[0.74778646,0.00011945865,0.22962046,0.00056360295,0.00008578966,0.0004030638,0.013649959,0.0051193964,0.002651865],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99945,0.00030328557,0.000015336973,0.00007242907,0.00011245864,0.000046462024],"domain_scores_gemma":[0.9980794,0.0010470889,0.00013097526,0.00036995384,0.00022283637,0.00014971376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028760922,0.0008053473,0.0007385292,0.0006079383,0.00047804086,0.0008587025,0.0022882463,0.0010114316,0.0039478173],"category_scores_gemma":[0.007579662,0.0006099104,0.0008783504,0.0004710686,0.0005832926,0.0011164694,0.0013386747,0.001194383,0.001052897],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044367366,0.00025357804,0.018774487,0.00021163729,0.00037386408,0.00018881718,0.0002480145,0.91226226,0.0031778733,0.023479212,0.017098038,0.023488546],"study_design_scores_gemma":[0.000055599314,0.000030262574,0.0009800623,0.000010363576,0.000007791582,0.000022509681,0.00001001253,0.9914743,0.0013849093,0.0035459641,0.0024690076,0.000009222532],"about_ca_topic_score_codex":0.008888797,"about_ca_topic_score_gemma":0.008128233,"teacher_disagreement_score":0.008888797,"about_ca_system_score_codex":0.00086759485,"about_ca_system_score_gemma":0.0010208484,"threshold_uncertainty_score":0.017674148},"labels":[],"label_agreement":null},{"id":"W4391263163","doi":"10.3847/1538-4357/ad0f21","title":"Mapping a Lower Limit on the Mass Fraction of the Cold Neutral Medium Using Fourier-transformed H i 21 cm Emission Line Spectra: Application to the DRAO Deep Field from DHIGLS and the HI4PI Survey","year":2024,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Algorithm; Computer science","score_opus":0.01636339598886917,"score_gpt":0.2504122139051132,"score_spread":0.23404881791624405,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391263163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6142485,0.0012412306,0.34339425,0.0010305828,0.00009053837,0.000103776125,0.0038433846,0.0069274637,0.029120266],"genre_scores_gemma":[0.914374,0.00029484724,0.08118761,0.00023607379,0.000089036366,0.00013037458,0.0015161964,0.0004649081,0.0017068991],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997552,0.000043542517,0.00000910016,0.00008622488,0.00006456196,0.000041433454],"domain_scores_gemma":[0.999292,0.00017905528,0.00019091828,0.00016481131,0.0000849797,0.0000882062],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000990681,0.0007988415,0.0005066692,0.0015985713,0.000342585,0.0011602622,0.0009041973,0.00060359976,0.0025873294],"category_scores_gemma":[0.0021441865,0.0004807058,0.00046184508,0.00085204083,0.00035352248,0.0009823813,0.0016724213,0.00070921035,0.0009901309],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0016956027,0.00017543322,0.14300683,0.0005439528,0.00037732846,0.00074619683,0.0012135238,0.048257723,0.52235794,0.034476984,0.0054294975,0.2417189],"study_design_scores_gemma":[0.00039487306,0.00025095855,0.37245965,0.00018239924,0.00027740645,0.0005623545,0.00061849033,0.3619731,0.18133153,0.049385417,0.032265708,0.00029817218],"about_ca_topic_score_codex":0.003684163,"about_ca_topic_score_gemma":0.0037518528,"teacher_disagreement_score":0.003684163,"about_ca_system_score_codex":0.0007609414,"about_ca_system_score_gemma":0.00030094382,"threshold_uncertainty_score":0.008655429},"labels":[],"label_agreement":null},{"id":"W4391322677","doi":"10.3847/1538-4357/ad1386","title":"AGN STORM 2. VI. Mapping Temperature Fluctuations in the Accretion Disk of Mrk 817","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"National Aeronautics and Space Administration; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Accretion disc; Astrophysics; Accretion (finance); Storm; Astronomy; Active galactic nucleus; Galaxy; Meteorology","score_opus":0.01251995185783606,"score_gpt":0.24292207296952895,"score_spread":0.2304021211116929,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391322677","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9962723,0.000024782245,0.0006946765,0.000045782275,0.000009731113,0.00000823621,0.00082533195,0.00039079762,0.0017284363],"genre_scores_gemma":[0.99679106,0.000015546448,0.0012642486,0.0000189714,0.000006395216,0.000007702555,0.0014138675,0.000081001825,0.00040115142],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999033,0.000012849464,0.0000044242297,0.000026799822,0.000020502703,0.00003213333],"domain_scores_gemma":[0.9997818,0.000050665447,0.000038403054,0.00004466288,0.000046694437,0.000037829777],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023562057,0.00034938296,0.0003175445,0.00031212147,0.00030894688,0.0005321925,0.0005690015,0.00049328373,0.0017671149],"category_scores_gemma":[0.00064188265,0.00016800368,0.000546855,0.00033082574,0.00015419038,0.00022128955,0.00022477227,0.00038612122,0.0006265565],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00081502786,0.00031140613,0.30409753,0.00014959944,0.00028671953,0.0012337036,0.00041645218,0.62519425,0.036527444,0.0013838727,0.0057455087,0.023838466],"study_design_scores_gemma":[0.0001019405,0.00021769156,0.26395395,0.00001664609,0.00005626463,0.00021443085,0.00015605814,0.7245416,0.0076274117,0.000362297,0.0027078267,0.000043808286],"about_ca_topic_score_codex":0.01179695,"about_ca_topic_score_gemma":0.012143399,"teacher_disagreement_score":0.01179695,"about_ca_system_score_codex":0.0005892389,"about_ca_system_score_gemma":0.00023142257,"threshold_uncertainty_score":0.023456573},"labels":[],"label_agreement":null},{"id":"W4391340894","doi":"10.3847/1538-4357/ad036e","title":"Probing the Subparsec Dust of a Supermassive Black Hole with the Tidal Disruption Event AT 2020mot","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"HORIZON EUROPE European Research Council; Israel Science Foundation; National Science Foundation","keywords":"Physics; Supermassive black hole; Astrophysics; Astronomy; Event (particle physics); Galaxy","score_opus":0.011899792809711042,"score_gpt":0.23344816352359274,"score_spread":0.2215483707138817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391340894","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99869967,0.000030097817,0.00014350048,0.00003281354,0.000005883738,0.0000053103513,0.0001620394,0.000012564335,0.00090818957],"genre_scores_gemma":[0.99942833,0.00001327858,0.00015004553,0.000018792673,0.000009217622,0.0000031088225,0.0001941798,0.000003039229,0.00018004948],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994063,0.0000054061575,0.0000023000919,0.000015713149,0.000014917231,0.000021105634],"domain_scores_gemma":[0.9997999,0.000024068531,0.00005549079,0.000014943721,0.000023433064,0.000082047154],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018852546,0.00017683735,0.00017816696,0.00047428085,0.0005281923,0.000376427,0.00024484764,0.0004517449,0.0012233141],"category_scores_gemma":[0.00033664232,0.00011408191,0.00020133254,0.0002276093,0.00021438736,0.00022516008,0.0005358653,0.00029709697,0.00028683],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033823212,0.00009665551,0.9393493,0.000020997626,0.000047459474,0.0019488459,0.0004901494,0.00044618314,0.05119444,0.00023729558,0.00045011335,0.0053802924],"study_design_scores_gemma":[0.000002459493,0.00005601802,0.99774504,0.00000235864,0.000005790361,0.0002604706,0.00012036282,0.00046379512,0.00096190354,0.000047143792,0.00033280943,0.0000018149145],"about_ca_topic_score_codex":0.002730037,"about_ca_topic_score_gemma":0.004730142,"teacher_disagreement_score":0.002730037,"about_ca_system_score_codex":0.00029118842,"about_ca_system_score_gemma":0.00007478473,"threshold_uncertainty_score":0.0054282546},"labels":[],"label_agreement":null},{"id":"W4391347680","doi":"10.3847/1538-4357/ad0cf7","title":"Reading between the (Spectral) Lines: Magellan/IMACS Spectroscopy of the Ultrafaint Dwarf Galaxies Eridanus IV and Centaurus I","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Argonne National Laboratory; SLAC National Accelerator Laboratory; Fondo Nacional de Desarrollo Científico y Tecnológico; Integrated Electronics Engineering Center, Binghamton University; Natural Sciences and Engineering Research Council of Canada; National Centre for Supercomputing Applications; Eidgenössische Technische Hochschule Zürich; Institut de Física d'Altes Energies; University of Sussex; Center for Cosmology and Astroparticle Physics, Ohio State University; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Deutsche Forschungsgemeinschaft; University of Illinois at Urbana-Champaign; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Yale University; University of Portsmouth; Kavli Institute for Cosmological Physics, University of Chicago; University of California, Santa Cruz; Ohio State University; University College London; National Aeronautics and Space Administration; U.S. Department of Energy; European Space Agency; Fermilab; Laboratory Directed Research and Development; National Science Foundation; Science and Technology Facilities Council","keywords":"Physics; Centaurus A; Astronomy; Astrophysics; Galaxy; Spectroscopy; Quasar; Spectral line; Active galactic nucleus","score_opus":0.00918471145754,"score_gpt":0.23580934489314861,"score_spread":0.22662463343560862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391347680","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98894894,0.00010132896,0.001066065,0.000062272484,0.000006856571,0.000004961437,0.001470941,0.00032207867,0.008016565],"genre_scores_gemma":[0.9947712,0.000027397533,0.0019807585,0.00002828823,0.000012066077,0.000004887239,0.0011626714,0.00003818986,0.0019744614],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998211,0.000014510002,0.000008942917,0.00006140164,0.000052673346,0.000041401978],"domain_scores_gemma":[0.9994912,0.00003890966,0.00016582932,0.00009044093,0.00012880017,0.00008478655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031508403,0.00018481682,0.000116968404,0.0016351583,0.0002874161,0.00057464564,0.0002958107,0.00017782142,0.004016173],"category_scores_gemma":[0.0005395771,0.000107311185,0.000131735,0.00082438317,0.00014282517,0.00029986468,0.0004892442,0.00013439784,0.0009898858],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003068126,0.000048127928,0.85557103,0.00006777779,0.000096535914,0.00012986377,0.0009730804,0.00084855733,0.07372963,0.0011821823,0.0045109824,0.06253532],"study_design_scores_gemma":[0.000004404051,0.000020698273,0.9818854,0.000007420495,0.000019153127,0.00007659483,0.00026624766,0.0008167163,0.01137818,0.000156679,0.0053594797,0.000009078351],"about_ca_topic_score_codex":0.0058945324,"about_ca_topic_score_gemma":0.011081076,"teacher_disagreement_score":0.0058945324,"about_ca_system_score_codex":0.00047774296,"about_ca_system_score_gemma":0.000118344426,"threshold_uncertainty_score":0.013435423},"labels":[],"label_agreement":null},{"id":"W4391347725","doi":"10.3847/1538-4357/ad148c","title":"An ALMA Spectroscopic Survey of the Brightest Submillimeter Galaxies in the SCUBA-2-COSMOS Field (AS2COSPEC): Physical Properties of z = 2–5 Ultra- and Hyperluminous Infrared Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Japan Society for the Promotion of Science; National Research Foundation; Science and Technology Facilities Council; Danmarks Grundforskningsfond; National Astronomical Observatory of Japan; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science and Technology Council; Academia Sinica; National Radio Astronomy Observatory; National Natural Science Foundation of China; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Star formation; Luminous infrared galaxy; Redshift; Luminosity; Infrared; Stellar mass; Astronomy; Spectral energy distribution","score_opus":0.012002071520376245,"score_gpt":0.22115917807089372,"score_spread":0.20915710655051747,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391347725","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99938583,0.000026493739,0.00003213281,0.0000063039442,6.2514727e-7,0.0000026215946,0.00023963727,0.000007208963,0.0002991067],"genre_scores_gemma":[0.99850476,0.000024529569,0.00014010405,0.0000145640215,0.000006448628,0.000004364729,0.0011310877,0.0000032990724,0.00017095331],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981123,0.000029095383,0.000011786512,0.000040945306,0.00004959298,0.00005741541],"domain_scores_gemma":[0.99907315,0.0000680689,0.00032267452,0.00008549845,0.00013473979,0.00031594795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003465586,0.0002840791,0.00022559353,0.0019929307,0.00035105553,0.00046296886,0.00021507879,0.00016464778,0.0012271672],"category_scores_gemma":[0.0004413575,0.00012923601,0.00020154094,0.00095038454,0.00020162838,0.0002603182,0.0004864432,0.00017346456,0.00034242318],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004255315,0.00003350062,0.9947589,0.000004397871,0.000017403625,0.000040400286,0.00008964367,0.00003352072,0.0032405043,0.000028116316,0.00019667222,0.0015144228],"study_design_scores_gemma":[0.0000024351014,0.000010450995,0.99950397,0.000001079627,0.0000035931025,0.00004107882,0.00004011843,0.0000829474,0.00017445625,0.0000046307823,0.00013436422,7.63713e-7],"about_ca_topic_score_codex":0.007182286,"about_ca_topic_score_gemma":0.0116313705,"teacher_disagreement_score":0.007182286,"about_ca_system_score_codex":0.0001945067,"about_ca_system_score_gemma":0.00016389781,"threshold_uncertainty_score":0.014280975},"labels":[],"label_agreement":null},{"id":"W4391388010","doi":"10.3847/1538-4357/ad11e1","title":"Evidence of Weak Circumstellar Medium Interaction in the Type II SN 2023axu","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Astrophysics Division; Heising-Simons Foundation; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; University of Leicester; College of Engineering, Michigan State University; University of North Carolina at Chapel Hill; California Institute of Technology; John Templeton Foundation; Science and Technology Facilities Council; Michigan State University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Type (biology)","score_opus":0.02568716870830339,"score_gpt":0.2821362811444505,"score_spread":0.2564491124361471,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391388010","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990932,0.000095802585,0.00011826892,0.000008964813,0.0000025326117,0.0000017690785,0.00009414,0.000009442992,0.000575936],"genre_scores_gemma":[0.99970007,0.000017318847,0.00005918277,0.000007117272,0.0000024982974,0.0000013805044,0.00013957854,0.000001991013,0.00007095156],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999379,0.000009298404,0.0000045807797,0.00001597633,0.000014592994,0.000017802022],"domain_scores_gemma":[0.9996954,0.00003639954,0.000112680165,0.0000188843,0.00002337377,0.000113196504],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001673884,0.00025136673,0.00025008613,0.00044900333,0.00041933838,0.0005487668,0.00019184718,0.00033144385,0.0009725671],"category_scores_gemma":[0.00030571598,0.00011488955,0.00020418483,0.00034595944,0.00027967503,0.00012324817,0.00032505224,0.00015020634,0.00030336998],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003029735,0.000052662203,0.97231764,0.0000192667,0.000031894364,0.0010560785,0.00010446556,0.00021963437,0.021972263,0.00021919413,0.00014393551,0.0035600425],"study_design_scores_gemma":[0.0000039907804,0.00008786887,0.99652857,0.0000043146797,0.000010036218,0.0011591322,0.0000935634,0.00068289245,0.00092227466,0.00012839034,0.00037508365,0.0000037958428],"about_ca_topic_score_codex":0.0031991927,"about_ca_topic_score_gemma":0.0041876193,"teacher_disagreement_score":0.0031991927,"about_ca_system_score_codex":0.00018763545,"about_ca_system_score_gemma":0.00011910759,"threshold_uncertainty_score":0.006361127},"labels":[],"label_agreement":null},{"id":"W4391402601","doi":"10.3847/1538-4357/ad0e69","title":"A Uniform Analysis of Debris Disks with the Gemini Planet Imager. I. An Empirical Search for Perturbations from Planetary Companions in Polarized Light Images","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Western University; National Research Council Canada; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Debris disk; Physics; Planet; Exoplanet; Planetary system; Astrophysics; Surface brightness; Brightness; Debris; Stars; Thick disk; Astronomy; Halo; Galaxy","score_opus":0.016102029613555082,"score_gpt":0.2747929398668307,"score_spread":0.2586909102532756,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391402601","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969472,0.00009211209,0.0015855579,0.000013941809,0.0000020730517,0.000018267778,0.00040296576,0.000032433087,0.0009054308],"genre_scores_gemma":[0.99755245,0.00003718505,0.0016885888,0.000006259509,0.0000048110405,0.000008074399,0.0005549533,0.000008805773,0.0001390581],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996445,0.000059051505,0.000035975492,0.00009402116,0.00011816582,0.00004823234],"domain_scores_gemma":[0.99884725,0.00023106756,0.0003098189,0.00018334642,0.0003109502,0.00011765366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055214646,0.00020505773,0.00014310818,0.0020654013,0.00044138817,0.0005480121,0.00015001724,0.00014643966,0.0007811673],"category_scores_gemma":[0.002239183,0.00011133148,0.00013507235,0.0009877303,0.00024418902,0.00039139873,0.0004940802,0.00013900783,0.000285405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020003121,0.000037232563,0.94326556,0.000016964445,0.000047052818,0.00018358103,0.00010412596,0.00039834145,0.038032938,0.000115776034,0.00022728869,0.01737111],"study_design_scores_gemma":[0.0000024329538,0.000028148099,0.99334514,0.0000024614449,0.000012999924,0.00031660576,0.00008589104,0.0020090984,0.0038392632,0.000039689316,0.00031586929,0.000002498753],"about_ca_topic_score_codex":0.0017838182,"about_ca_topic_score_gemma":0.0028530634,"teacher_disagreement_score":0.0020654013,"about_ca_system_score_codex":0.00018805062,"about_ca_system_score_gemma":0.00011850626,"threshold_uncertainty_score":0.0035469532},"labels":[],"label_agreement":null},{"id":"W4391437318","doi":"10.3847/1538-4357/ad1932","title":"Detection of CO(1−0) Emission at the Tips of the Tidal Tail in the Antennae Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Galaxy; Astronomy; Astrophysics; Emission spectrum; Radio galaxy; Spectral line","score_opus":0.009627754525032752,"score_gpt":0.24112270027541108,"score_spread":0.23149494575037832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391437318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988772,0.000044577682,0.00037525338,0.0000063562247,0.0000014923602,0.0000035554986,0.00009550204,0.000025481459,0.0005705364],"genre_scores_gemma":[0.999458,0.000011089317,0.0002478551,0.000009315113,0.0000021890223,0.0000021960398,0.00009969589,0.0000027465921,0.00016687022],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991417,0.0000082157185,0.000004361588,0.000033662513,0.000015673462,0.00002393549],"domain_scores_gemma":[0.9996007,0.00004483153,0.00009396147,0.000043870677,0.00006012249,0.00015642309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013490822,0.00016923105,0.00015867858,0.00076741085,0.00028323833,0.00036080892,0.00021302278,0.0002665874,0.0008621279],"category_scores_gemma":[0.0002620149,0.0001656024,0.0001440166,0.00037989195,0.00030558105,0.00016486317,0.000338031,0.00017072262,0.00026995954],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008180648,0.000022926211,0.86114985,0.000014232573,0.000026253363,0.00020745446,0.00028634092,0.00011610291,0.13317072,0.000059893264,0.00010826183,0.0047561266],"study_design_scores_gemma":[0.0000017572889,0.000028888051,0.99672216,0.0000011375726,0.0000062260438,0.00013366289,0.00006266877,0.000150078,0.0026728846,0.000012913956,0.00020488967,0.0000028120792],"about_ca_topic_score_codex":0.0024171635,"about_ca_topic_score_gemma":0.003938977,"teacher_disagreement_score":0.0024171635,"about_ca_system_score_codex":0.00016099545,"about_ca_system_score_gemma":0.00006211858,"threshold_uncertainty_score":0.004806161},"labels":[],"label_agreement":null},{"id":"W4391448551","doi":"10.3847/1538-4357/ad1243","title":"Validation of Elemental and Isotopic Abundances in Late-M Spectral Types with the Benchmark HIP 55507 AB System","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"National Aeronautics and Space Administration; Heising-Simons Foundation; National Science Foundation","keywords":"Physics; Astrophysics; Benchmark (surveying); Astronomy; Geodesy","score_opus":0.00454982463746512,"score_gpt":0.200591088595177,"score_spread":0.19604126395771188,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391448551","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99300355,0.00007072832,0.00096231373,0.000025066744,0.000015022078,0.00001585569,0.0029298041,0.00047075935,0.0025069735],"genre_scores_gemma":[0.98901117,0.000023814397,0.0018583064,0.000051220526,0.000012032783,0.000013873048,0.00846823,0.000103667626,0.00045767965],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99961287,0.00004503601,0.000023530562,0.00017001243,0.00008662468,0.0000620289],"domain_scores_gemma":[0.9994474,0.000060900453,0.000066912915,0.00015113555,0.00017613864,0.000097465774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006371618,0.00038399658,0.00022246366,0.00083454105,0.0005169846,0.00064024347,0.0005349156,0.00031484143,0.0015015805],"category_scores_gemma":[0.0010036664,0.00014136323,0.00031401555,0.000610971,0.00030439615,0.00035482566,0.0007664257,0.00017839271,0.0014312636],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018093378,0.00034182522,0.8129452,0.00015924951,0.00029997824,0.00051308854,0.0005130626,0.017812742,0.1107544,0.001304103,0.011664874,0.04188216],"study_design_scores_gemma":[0.00012869936,0.0004845206,0.88242996,0.0000320628,0.00013351066,0.00030647332,0.00037490606,0.046363823,0.05743817,0.0005737715,0.011695085,0.00003886998],"about_ca_topic_score_codex":0.019935599,"about_ca_topic_score_gemma":0.013058359,"teacher_disagreement_score":0.019935599,"about_ca_system_score_codex":0.0005788943,"about_ca_system_score_gemma":0.00018657447,"threshold_uncertainty_score":0.039639115},"labels":[],"label_agreement":null},{"id":"W4391448937","doi":"10.3847/1538-4357/ad0cf0","title":"Cosmic Tidal Reconstruction in Redshift Space","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Key Research and Development Program of China; Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China","keywords":"Physics; Redshift; COSMIC cancer database; Astronomy; Space (punctuation); Astrophysics; Cosmic ray; Galaxy","score_opus":0.00874076649826365,"score_gpt":0.22979921085852914,"score_spread":0.2210584443602655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391448937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93971086,0.00008654692,0.05699097,0.00015980245,0.000016739337,0.00001069118,0.0004097352,0.00040186977,0.0022129342],"genre_scores_gemma":[0.9934435,0.000025224594,0.0058049415,0.000012881877,0.000003863292,0.0000022753266,0.00028094524,0.000046180678,0.00038017493],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998228,0.000051435985,0.000008996352,0.00003631101,0.000056157216,0.000024397388],"domain_scores_gemma":[0.9990953,0.0002549411,0.00017814738,0.00020415893,0.00020153406,0.000065934335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005582104,0.00026796755,0.00018447475,0.00061697717,0.00017074868,0.00054255873,0.00031005222,0.0002505637,0.0011397516],"category_scores_gemma":[0.003784217,0.0001726621,0.00028756986,0.0005787142,0.00041794416,0.00041801672,0.000412671,0.00026625823,0.00017518293],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030644564,0.00004374655,0.08361244,0.000046465706,0.000106817075,0.00015177423,0.00017578503,0.84973633,0.019350948,0.015945958,0.00063291215,0.029890396],"study_design_scores_gemma":[0.000020030771,0.000024289253,0.030493632,0.000006008326,0.000012668346,0.00007048701,0.000036804024,0.9601807,0.0048868502,0.0035887144,0.00065906456,0.000020739513],"about_ca_topic_score_codex":0.008053081,"about_ca_topic_score_gemma":0.004585975,"teacher_disagreement_score":0.008053081,"about_ca_system_score_codex":0.0005488871,"about_ca_system_score_gemma":0.0002927696,"threshold_uncertainty_score":0.01601243},"labels":[],"label_agreement":null},{"id":"W4391462058","doi":"10.3847/1538-4357/ad40aa","title":"Polarization Properties of 128 Nonrepeating Fast Radio Bursts from the First CHIME/FRB Baseband Catalog","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; University of British Columbia; York University; Perimeter Institute; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Foundation for Innovation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Baseband; Polarization (electrochemistry); Astronomy; Astrophysics","score_opus":0.012353536551633598,"score_gpt":0.26541091092874347,"score_spread":0.25305737437710984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391462058","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922948,0.00023703171,0.00041007015,0.000041147574,0.0000057642033,0.000021549085,0.0053077578,0.00013872745,0.0015430708],"genre_scores_gemma":[0.965015,0.0002375174,0.0016975937,0.00005168979,0.000036700592,0.000038559476,0.03133735,0.00007929823,0.0015061607],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996996,0.000018700004,0.000014798789,0.00006322897,0.000107019645,0.000096673124],"domain_scores_gemma":[0.9988827,0.00016287636,0.00027722245,0.00018704557,0.00025842956,0.00023177409],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034882952,0.00039301507,0.00036276778,0.0031793402,0.00035006125,0.0005514811,0.0002754445,0.0002684982,0.002379056],"category_scores_gemma":[0.0010310502,0.00020486834,0.00034031723,0.0019822961,0.00018250944,0.0001856809,0.00051210116,0.0003037213,0.0012255843],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000437892,0.00010267465,0.88245773,0.00008488397,0.0001433157,0.0005201014,0.00037154765,0.0012700302,0.055620473,0.00010890547,0.0038207842,0.05506171],"study_design_scores_gemma":[0.0000072356424,0.000013222181,0.9971329,0.000003886058,0.00001128233,0.00013411426,0.00003796633,0.00030169782,0.0010220176,0.00001464531,0.0013155295,0.0000054824677],"about_ca_topic_score_codex":0.0085466085,"about_ca_topic_score_gemma":0.009172959,"teacher_disagreement_score":0.0085466085,"about_ca_system_score_codex":0.00033050482,"about_ca_system_score_gemma":0.00017578278,"threshold_uncertainty_score":0.016993761},"labels":[],"label_agreement":null},{"id":"W4391533177","doi":"10.3847/1538-4357/ad1193","title":"Spectroscopic r-process Abundance Retrieval for Kilonovae. II. Lanthanides in the Inferred Abundance Patterns of Multicomponent Ejecta from the GW170817 Kilonova","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; University of Toronto; Bishop's University; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Kilonova; Physics; Ejecta; Nucleosynthesis; Astrophysics; Abundance (ecology); r-process; Astronomy; Supernova; Biology","score_opus":0.017059614691695445,"score_gpt":0.2770965964369806,"score_spread":0.26003698174528517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391533177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927194,0.00022956678,0.0028282541,0.000059568916,0.000016490909,0.000012188239,0.001578505,0.00055723364,0.0019987398],"genre_scores_gemma":[0.9871471,0.00010992966,0.0075300992,0.000033658893,0.000013013915,0.00001335851,0.0041757533,0.00022752835,0.0007495661],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999254,0.0000037425295,0.0000030936071,0.000025582327,0.000023577593,0.00001859912],"domain_scores_gemma":[0.9998281,0.000023415963,0.000045089375,0.000027985605,0.000042834334,0.00003261804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021633336,0.0004597216,0.00022394783,0.001324772,0.00029282682,0.00045215202,0.0003504097,0.00038198696,0.00089595316],"category_scores_gemma":[0.00048460928,0.00024563022,0.000642443,0.0005907124,0.00012755419,0.0004383641,0.00055944634,0.00029567198,0.00040124307],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012168948,0.0001044814,0.41928026,0.00021962276,0.00031441165,0.0017408818,0.00064775965,0.0065022265,0.51581174,0.00074382,0.0027103967,0.050707508],"study_design_scores_gemma":[0.000062788495,0.0001131378,0.86042,0.000039007984,0.00017123244,0.00097157,0.00039452687,0.052904844,0.077051856,0.0006434903,0.007159618,0.00006796634],"about_ca_topic_score_codex":0.004549013,"about_ca_topic_score_gemma":0.01074491,"teacher_disagreement_score":0.004549013,"about_ca_system_score_codex":0.00032758867,"about_ca_system_score_gemma":0.00020209147,"threshold_uncertainty_score":0.009045124},"labels":[],"label_agreement":null},{"id":"W4391539716","doi":"10.3847/1538-4357/ad14f8","title":"Mid-infrared Variability of Young Stellar Objects on Timescales of Days to Years","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea","keywords":"Physics; Astrophysics; Young stellar object; Brightness; Photosphere; Astronomy; Accretion (finance); Starspot; Amplitude; Star formation; Light curve; Stars; Spectral line","score_opus":0.0084823498790558,"score_gpt":0.24083266806450498,"score_spread":0.23235031818544918,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391539716","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99899083,0.000079303136,0.00019650788,0.000008164654,0.000002446982,0.000002230256,0.00033765522,0.000011705838,0.00037116668],"genre_scores_gemma":[0.99885726,0.000027294214,0.00015401296,0.000005806797,0.000008270283,0.000004036153,0.00082548003,0.000004030418,0.00011387783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985516,0.000011158939,0.00001285658,0.000052732335,0.00003402536,0.00003413463],"domain_scores_gemma":[0.9990262,0.00019759787,0.00044044593,0.0000917111,0.00011363388,0.00013047113],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039718376,0.000119337696,0.0001587329,0.0012030848,0.00015340887,0.00045673436,0.00017594107,0.00019683111,0.00065353775],"category_scores_gemma":[0.0010644292,0.00007364364,0.00022592951,0.00064189587,0.00015167697,0.00040173333,0.0004326585,0.00016446295,0.00019807804],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007697335,0.000028870487,0.98397315,0.000011742638,0.0000520723,0.000057394303,0.0000858022,0.00042565356,0.010359104,0.00010248897,0.00017411482,0.00465274],"study_design_scores_gemma":[5.2573284e-7,0.000011348994,0.9992132,0.0000011773124,0.0000044512226,0.00002577132,0.000023489167,0.00033289412,0.00026948922,0.000022761422,0.00009351738,0.0000013734698],"about_ca_topic_score_codex":0.00089145073,"about_ca_topic_score_gemma":0.0010279425,"teacher_disagreement_score":0.0012030848,"about_ca_system_score_codex":0.00014206821,"about_ca_system_score_gemma":0.000053199226,"threshold_uncertainty_score":0.0021862984},"labels":[],"label_agreement":null},{"id":"W4391540038","doi":"10.3847/1538-4357/ad165e","title":"The One-hundred-deg<sup>2</sup> DECam Imaging in Narrowbands (ODIN): Survey Design and Science Goals","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Institut de Física d'Altes Energies; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Ministry of Science and ICT, South Korea; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Deutsche Forschungsgemeinschaft; University of Sussex; National Research Foundation of Korea; University of Portsmouth; Universidad Andrés Bello; Purdue Research Foundation; University of Chicago; National Research Foundation; Ohio State University; University of Illinois at Urbana-Champaign; Nuclear Safety and Security Commission; Ministério da Ciência, Tecnologia e Inovação; University College London; National Aeronautics and Space Administration; Purdue University; Science and Technology Facilities Council; U.S. Department of Energy; Fermilab; National Science Foundation","keywords":"Narrowband; Physics; Redshift; Galaxy; Astrophysics; Dark energy; Sky; Astronomy; Halo; Optics; Cosmology","score_opus":0.014010982962858187,"score_gpt":0.24277482180103677,"score_spread":0.22876383883817858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391540038","genre_codex":"empirical","genre_gemma":"protocol","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"protocol","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.53992516,0.0054080137,0.29597202,0.013592122,0.0005185208,0.009863793,0.032182265,0.0040125065,0.098525606],"genre_scores_gemma":[0.42064914,0.0017732799,0.5157792,0.00589893,0.00046455197,0.009067451,0.0279378,0.0006231037,0.017806543],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99856263,0.0004136527,0.000058504724,0.00023654406,0.00044450676,0.0002842123],"domain_scores_gemma":[0.99650806,0.0004038007,0.00044295934,0.00040230106,0.001147216,0.0010956795],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0064228545,0.0007183032,0.0003898706,0.0009867192,0.00077929103,0.0020332895,0.0010441636,0.0009438845,0.0020135525],"category_scores_gemma":[0.0025174625,0.00058742793,0.0003595265,0.0007958733,0.0006616665,0.0011668318,0.0020461592,0.0007626721,0.0016023361],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0036366966,0.00080726465,0.3860515,0.0012121542,0.00018135927,0.0003694535,0.00087168417,0.00960509,0.10592868,0.036452446,0.05107602,0.4038076],"study_design_scores_gemma":[0.00059048505,0.0027315964,0.51988244,0.00039578427,0.0002107619,0.00090422423,0.001623621,0.026490545,0.073205724,0.01655907,0.3572336,0.00017214307],"about_ca_topic_score_codex":0.00405885,"about_ca_topic_score_gemma":0.011033414,"teacher_disagreement_score":0.0064228545,"about_ca_system_score_codex":0.0015686891,"about_ca_system_score_gemma":0.0023849788,"threshold_uncertainty_score":0.033967674},"labels":[],"label_agreement":null},{"id":"W4391591775","doi":"10.3847/1538-4357/ad4152","title":"Fast and Slow Crystallization-driven Convection in White Dwarfs","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; National Aeronautics and Space Administration","keywords":"White dwarf; Crystallization; Convection; Astrophysics; Physics; Astronomy; Geology; Geophysics; Mechanics; Stars; Thermodynamics","score_opus":0.009479626523962587,"score_gpt":0.22651564207834032,"score_spread":0.21703601555437774,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391591775","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99526644,0.00007774676,0.0035828885,0.000045762885,0.00000547469,0.0000067518667,0.000032216918,0.000046431753,0.00093639124],"genre_scores_gemma":[0.99934787,0.000019391204,0.00043553967,0.000005515194,0.000004871623,0.0000029371254,0.00002250595,0.000011885617,0.00014955673],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999205,0.000020107986,0.0000044275303,0.000016587293,0.000016061356,0.000022262118],"domain_scores_gemma":[0.9997892,0.00006545992,0.000041184503,0.000022819939,0.00003534091,0.00004592277],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030816524,0.0003863132,0.00037707275,0.00037036632,0.000440843,0.00056159735,0.00032622766,0.00036011616,0.00035192407],"category_scores_gemma":[0.00064556004,0.00018581054,0.00044739177,0.0002190948,0.00069484,0.00040852357,0.00055507215,0.00025300338,0.00006452572],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036233678,0.00013141315,0.08013243,0.000083323386,0.00012881953,0.00075681345,0.00056033366,0.69461536,0.1980039,0.018770736,0.0003916274,0.0060628536],"study_design_scores_gemma":[0.000080537466,0.00006525053,0.02085217,0.000004706379,0.000012727891,0.0000573467,0.00007640559,0.9592453,0.015586652,0.0035523751,0.00044756802,0.000018871786],"about_ca_topic_score_codex":0.0074692075,"about_ca_topic_score_gemma":0.002904047,"teacher_disagreement_score":0.0074692075,"about_ca_system_score_codex":0.0008938254,"about_ca_system_score_gemma":0.00044931716,"threshold_uncertainty_score":0.014851451},"labels":[],"label_agreement":null},{"id":"W4391598467","doi":"10.3847/1538-4357/ad0558","title":"Two of a Kind: Comparing Big and Small Black Holes in Binaries with Gravitational Waves","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Science Foundation","keywords":"Physics; Binary number; Gravitational wave; Astrophysics; Black hole (networking); Population; Stars; Binary black hole; Binary star; Mass distribution; Galaxy","score_opus":0.0215003146607077,"score_gpt":0.3059091953372018,"score_spread":0.2844088806764941,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391598467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988417,0.000038776467,0.0004977508,0.000044717246,0.0000050953277,0.000007659008,0.000051024057,0.0000094750085,0.0005037904],"genre_scores_gemma":[0.99971503,0.0000069299845,0.00012673449,0.000013624059,0.000004476648,0.0000019525269,0.000066999746,0.0000044143317,0.00005974217],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99961615,0.00015712809,0.00002369591,0.00006587918,0.00005878513,0.000078394565],"domain_scores_gemma":[0.9960078,0.0026569767,0.0003868934,0.00017493285,0.00022745265,0.0005458351],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014120741,0.00040445913,0.0005818218,0.0015283957,0.0007329164,0.0015982199,0.0005093866,0.0007106582,0.0023744567],"category_scores_gemma":[0.005531006,0.00015672839,0.00033186754,0.00089744834,0.00094222714,0.0014490023,0.0014170383,0.0005174337,0.0002863101],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0022434678,0.00050906884,0.9552788,0.00005934979,0.0002768638,0.0003880524,0.00090293965,0.018826302,0.004371379,0.006391484,0.00072557287,0.0100267995],"study_design_scores_gemma":[0.00012149405,0.0004345992,0.81775063,0.00002142169,0.00011613912,0.00029822675,0.0025585112,0.15901887,0.0027849996,0.016133457,0.00070127076,0.000060216684],"about_ca_topic_score_codex":0.004961188,"about_ca_topic_score_gemma":0.003406455,"teacher_disagreement_score":0.004961188,"about_ca_system_score_codex":0.00059645216,"about_ca_system_score_gemma":0.00026855682,"threshold_uncertainty_score":0.009864628},"labels":[],"label_agreement":null},{"id":"W4391613427","doi":"10.3847/1538-4357/ad18c5","title":"A Cacophony of Echoes from Daily Monitoring of the Crab Pulsar at Jodrell Bank","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geophysics and Gravity Measurements","field":"Earth and Planetary Sciences","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Science and Technology Facilities Council","keywords":"Physics; Pulsar; Astronomy; Crab Pulsar; Astrophysics","score_opus":0.016047164385689816,"score_gpt":0.21345193095787793,"score_spread":0.1974047665721881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391613427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9932794,0.00007731757,0.00047153185,0.00003581207,0.000015145286,0.000014109583,0.0037169761,0.000073983734,0.0023157974],"genre_scores_gemma":[0.99245983,0.000074075615,0.001518931,0.000027556402,0.000019621759,0.000015982207,0.004470722,0.000037531892,0.0013756892],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999864,0.000013113683,0.0000096673575,0.0000331876,0.000055198347,0.00002486139],"domain_scores_gemma":[0.999243,0.000108347056,0.0001835076,0.00010122343,0.00020033927,0.00016356487],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023274917,0.00016348512,0.00013107253,0.0019004542,0.000326668,0.000510729,0.00014965264,0.00024145875,0.0015332521],"category_scores_gemma":[0.00078734703,0.00013104042,0.00012738342,0.0010938576,0.00016094433,0.00015143563,0.0004474496,0.00024268526,0.000611718],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024362706,0.000052371433,0.92633885,0.00006697917,0.000080700745,0.0005076963,0.0010822243,0.0005489642,0.043616686,0.00014400341,0.0024688973,0.024849035],"study_design_scores_gemma":[0.0000015776955,0.000012670788,0.9977761,0.000004030927,0.000005032176,0.00006956232,0.00010095605,0.00020472915,0.00083237566,0.00000862168,0.0009804715,0.0000038066235],"about_ca_topic_score_codex":0.012858929,"about_ca_topic_score_gemma":0.05461876,"teacher_disagreement_score":0.012858929,"about_ca_system_score_codex":0.00022625396,"about_ca_system_score_gemma":0.00023418896,"threshold_uncertainty_score":0.025568187},"labels":[],"label_agreement":null},{"id":"W4391646746","doi":"10.3847/1538-4357/ad1387","title":"The EDGE-CALIFA Survey: Molecular Gas and Star Formation Activity across the Green Valley","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Agencia Nacional de Investigación y Desarrollo; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Star formation; Stellar mass; Galaxy formation and evolution; Surface brightness; Astronomy","score_opus":0.010273872476359396,"score_gpt":0.239084380399159,"score_spread":0.2288105079227996,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391646746","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99411833,0.00008366589,0.000044063858,0.000047006935,0.0000018072176,0.0000051792244,0.0030000205,0.000018361596,0.0026815976],"genre_scores_gemma":[0.9936092,0.00008975687,0.0001799799,0.0000458707,0.00000769333,0.0000068332442,0.0051760124,0.000011543242,0.0008731581],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998568,0.000013596707,0.000003860646,0.000052994226,0.000037622387,0.000035093315],"domain_scores_gemma":[0.999178,0.000083966144,0.00015715345,0.00008347734,0.00021335376,0.00028405027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001547411,0.000117284144,0.00020764598,0.0012687686,0.00043272655,0.0007139879,0.00031878756,0.0001546905,0.002339331],"category_scores_gemma":[0.00042762718,0.0001015842,0.00011538646,0.0013694469,0.00023233722,0.0002075935,0.00054077595,0.00020194643,0.00035924913],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000083594176,0.000026138032,0.99341583,0.000009628234,0.000022296232,0.00004295781,0.00016764345,0.000059340942,0.0012146733,0.00008170726,0.0015567781,0.0033193056],"study_design_scores_gemma":[0.0000039082115,0.0000054656093,0.9991326,0.0000030764143,0.000004048709,0.000014888612,0.000092832226,0.0000864334,0.00006936301,0.0000088218585,0.000577659,0.0000010474421],"about_ca_topic_score_codex":0.14090273,"about_ca_topic_score_gemma":0.34367946,"teacher_disagreement_score":0.14090273,"about_ca_system_score_codex":0.0005411928,"about_ca_system_score_gemma":0.00042211916,"threshold_uncertainty_score":0.28016514},"labels":[],"label_agreement":null},{"id":"W4391682745","doi":"10.3847/1538-4357/ad1033","title":"CLASSY. VIII. Exploring the Source of Ionization with UV Interstellar Medium Diagnostics in Local High-z Analogs*","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Fundação para a Ciência e a Tecnologia; Science and Technology Facilities Council; Office of Science; Agencia Nacional de Investigación y Desarrollo; Leibniz-Institut für Astrophysik Potsdam; Space Telescope Science Institute; European Southern Observatory; York University; Istituto Nazionale di Astrofisica; Arizona Board of Regents; Leibniz-Gemeinschaft; University of Notre Dame; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Ministero dell’Istruzione, dell’Università e della Ricerca; Carnegie Mellon University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; University of Minnesota; National Science Foundation; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Physics; Interstellar medium; Ionization; Astrochemistry; Astronomy; Astrophysics; Ion; Galaxy; Quantum mechanics","score_opus":0.008552320248284832,"score_gpt":0.19609417374450067,"score_spread":0.18754185349621583,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391682745","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9872062,0.0001412327,0.0012865007,0.00006277278,0.000008697672,0.000012081038,0.004166661,0.0001322394,0.006983589],"genre_scores_gemma":[0.99616444,0.000034118824,0.0009117257,0.000017673048,0.000004816187,0.0000062754684,0.0021122207,0.000026367848,0.0007224084],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999138,0.000007822866,0.0000037885086,0.00003440535,0.000014180032,0.000025996938],"domain_scores_gemma":[0.9994217,0.00007087946,0.00022603862,0.000056876826,0.00010727843,0.00011736061],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017818836,0.00015965887,0.00012093968,0.0016856776,0.0002929301,0.0008402618,0.00015205274,0.00016846776,0.004128469],"category_scores_gemma":[0.00055195705,0.000048876143,0.00015199259,0.00076559646,0.00017118442,0.00034043,0.00060314115,0.0001731019,0.0008779203],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016363745,0.000026401813,0.9501406,0.00004701715,0.000034842687,0.00009292517,0.00028010624,0.00047698343,0.007192853,0.0009585486,0.001975435,0.03861062],"study_design_scores_gemma":[0.0000031617767,0.000024344878,0.9934668,0.0000084373005,0.000006747987,0.00009580425,0.00030887613,0.00092258904,0.0013231823,0.00025022714,0.0035871374,0.0000027798415],"about_ca_topic_score_codex":0.0077852462,"about_ca_topic_score_gemma":0.008427995,"teacher_disagreement_score":0.0077852462,"about_ca_system_score_codex":0.00036952939,"about_ca_system_score_gemma":0.00014718063,"threshold_uncertainty_score":0.015479863},"labels":[],"label_agreement":null},{"id":"W4391683517","doi":"10.3847/1538-4357/ad0fd8","title":"High-spectral-resolution Observations of the Optical Filamentary Nebula Surrounding NGC 1275","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McGill University; University of Waterloo; Université Laval; Centre for Research in Astrophysics of Québec; Université de Montréal","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministerio de Ciencia e Innovación; Université de Montréal; Nuclear Safety and Security Commission; Centre National de la Recherche Scientifique; Institut national des sciences de l'Univers; Grantová Agentura České Republiky; Agencia Estatal de Investigación; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Nebula; Spectral resolution; Emission nebula; High resolution; Protoplanetary nebula; Spectral line; Stars; Remote sensing","score_opus":0.020241692897098342,"score_gpt":0.23633414682302853,"score_spread":0.21609245392593018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391683517","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99484587,0.00019952007,0.00064369576,0.000021412618,0.0000050692993,0.000005470738,0.0006106272,0.0000826273,0.0035856122],"genre_scores_gemma":[0.99769115,0.000046682453,0.0008805347,0.000015897105,0.0000059140807,0.0000030440376,0.0008622985,0.0000073378487,0.00048717635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999405,0.0000033817605,0.0000026185335,0.000015234354,0.000023353829,0.000014824564],"domain_scores_gemma":[0.99989676,0.0000084817675,0.000022486314,0.0000118399785,0.000018347722,0.000041972926],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011431266,0.00013938239,0.000118709955,0.00076388096,0.00028090028,0.0002922414,0.00020391498,0.0001240872,0.0013383279],"category_scores_gemma":[0.00013391518,0.00008516919,0.00013264772,0.00039748524,0.00013146983,0.00015159657,0.0002933474,0.00013617547,0.00022981175],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00043019062,0.00015170671,0.5642325,0.00013944524,0.00022937098,0.0015644071,0.0007647384,0.0022677248,0.36914262,0.0006108728,0.0046778563,0.055788554],"study_design_scores_gemma":[0.00001221053,0.00004590056,0.9908824,0.0000127736275,0.00002107166,0.00025933114,0.000113179456,0.0009342,0.0044623753,0.0000594164,0.003190199,0.0000069597195],"about_ca_topic_score_codex":0.013689807,"about_ca_topic_score_gemma":0.02950409,"teacher_disagreement_score":0.013689807,"about_ca_system_score_codex":0.0004052986,"about_ca_system_score_gemma":0.00012274596,"threshold_uncertainty_score":0.02722025},"labels":[],"label_agreement":null},{"id":"W4391684587","doi":"10.3847/1538-4357/ad17ba","title":"First Detection of Polarization in X-Rays for PSR B0540-69 and Its Nebula","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Istituto Nazionale di Astrofisica; Nuclear Safety and Security Commission; Agenzia Spaziale Italiana; Hong Kong Government; National Natural Science Foundation of China; National Key Research and Development Program of China; Oak Ridge Associated Universities; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Polarization (electrochemistry); Astrophysics; Pulsar; Pulsar wind nebula; Nebula; Crab Nebula; Polarimetry; Large Magellanic Cloud; Astronomy; Stars; Optics; Scattering","score_opus":0.011269009823086354,"score_gpt":0.23228099027433846,"score_spread":0.22101198045125212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391684587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99754363,0.00011986309,0.00045536674,0.000021474552,0.0000068609374,0.000007115031,0.0002604081,0.000041819032,0.0015433967],"genre_scores_gemma":[0.99811125,0.00006841231,0.0006140528,0.00004194935,0.000010891334,0.0000061321625,0.00076154014,0.000012709384,0.00037307304],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99984443,0.000012270943,0.0000051530997,0.000038087655,0.000057881996,0.00004216852],"domain_scores_gemma":[0.9997582,0.00002909481,0.000057996906,0.000025280418,0.00004965793,0.00007971525],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015192752,0.00021539441,0.00022489362,0.0007225158,0.00037864043,0.00045320904,0.00024225016,0.00033780272,0.0012578382],"category_scores_gemma":[0.000315516,0.00019655318,0.0001705292,0.0004916101,0.00022635733,0.00017749415,0.00051936356,0.0003677692,0.00026971975],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008181484,0.00019361249,0.28871942,0.00010278349,0.00010132711,0.0009521347,0.0003108246,0.0003149093,0.67380077,0.00029514413,0.00083579763,0.03355514],"study_design_scores_gemma":[0.000014710869,0.00028300847,0.9575694,0.0000111246145,0.000025700367,0.0007935773,0.0001107301,0.0006929408,0.037698377,0.00010753886,0.0026806016,0.000012158485],"about_ca_topic_score_codex":0.0015245366,"about_ca_topic_score_gemma":0.0022656077,"teacher_disagreement_score":0.0015245366,"about_ca_system_score_codex":0.00019942237,"about_ca_system_score_gemma":0.00010920451,"threshold_uncertainty_score":0.004207909},"labels":[],"label_agreement":null},{"id":"W4391753163","doi":"10.3847/1538-4357/ad04d7","title":"SN 2022oqm–A Ca-rich Explosion of a Compact Progenitor Embedded in C/O Circumstellar Material","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"University of California Observatories; Stockholms Universitet; Helen Kimmel Center for Planetary Sciences, Weizmann Institute of Science; Deutsches Elektronen-Synchrotron; Liverpool John Moores University; Israel Science Foundation; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Weizmann Institute of Science; Deutsche Forschungsgemeinschaft; Trinity College Dublin; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet; Northwestern University; University of Warwick; Alexander Family Foundation; National Science Foundation; University of Washington; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; University of Leicester; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation","keywords":"Physics; Astrophysics; Light curve; Ejecta; Supernova; White dwarf; RADIUS; Spectral line; Emission spectrum; Astronomy; Stars","score_opus":0.012621386488783116,"score_gpt":0.24862015078388636,"score_spread":0.23599876429510325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391753163","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984503,0.00014553544,0.00023649038,0.000022576798,0.000008049859,0.000013196174,0.00012675003,0.000010298639,0.000986679],"genre_scores_gemma":[0.99853384,0.00007242593,0.00035263144,0.000040422085,0.000015858028,0.000005075012,0.00042182588,0.000003365121,0.00055453915],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999219,0.00000444423,0.000003831114,0.000021913767,0.00002025332,0.00002766076],"domain_scores_gemma":[0.9999273,0.0000061003852,0.000017125603,0.000008007823,0.000009073525,0.000032385484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001838063,0.00043933443,0.0002585181,0.00040132893,0.00039951692,0.0004903086,0.00021954377,0.00043131976,0.0007769968],"category_scores_gemma":[0.00016891315,0.00012496326,0.00021667521,0.00023619864,0.00022370157,0.00017889912,0.00046856963,0.00019601699,0.0002808826],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001146475,0.0002553024,0.57714784,0.00012466604,0.00013601423,0.033085648,0.00031595078,0.001056896,0.36281776,0.0017666531,0.0011375779,0.021009257],"study_design_scores_gemma":[0.000054598015,0.000809434,0.93386304,0.000029655508,0.000052983654,0.025452642,0.0003814587,0.0038133464,0.023432964,0.00090417074,0.011180367,0.000025178337],"about_ca_topic_score_codex":0.0015844875,"about_ca_topic_score_gemma":0.001665457,"teacher_disagreement_score":0.0015844875,"about_ca_system_score_codex":0.00023957787,"about_ca_system_score_gemma":0.000113902766,"threshold_uncertainty_score":0.0031505227},"labels":[],"label_agreement":null},{"id":"W4391753920","doi":"10.3847/1538-4357/ad16e4","title":"Stellar Population Properties in the Stellar Streams aroundSPRC047","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Division of Astronomical Sciences; Agencia Estatal de Investigación; Natural Sciences and Engineering Research Council of Canada; Office of Science; Instituto de Astrofísica de Andalucía; Ministerio de Economía y Competitividad; Centre National de la Recherche Scientifique; Universidad Internacional de La Rioja; Chinese Academy of Sciences; Deutsche Forschungsgemeinschaft; Ministerio de Ciencia, Innovación y Universidades; University of Sussex; National Energy Research Scientific Computing Center; Jet Propulsion Laboratory; Ministry of Education, Culture, Sports, Science and Technology; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; Junta de Andalucía; National Science Foundation","keywords":"Physics; Astrophysics; Stellar population; Galaxy; Metallicity; Surface brightness; Population; Spectral energy distribution; Brightness; Flux (metallurgy); Star formation; Astronomy","score_opus":0.011749913465909196,"score_gpt":0.21557558199243096,"score_spread":0.20382566852652176,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391753920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991352,0.0000304297,0.00033576164,0.000006694681,0.0000013672989,0.0000034655318,0.00014090855,0.000028841601,0.00031738062],"genre_scores_gemma":[0.99857366,0.00001895105,0.0004983537,0.0000064267924,0.000003216798,0.0000032311657,0.0006745123,0.000016829279,0.00020476016],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999014,0.000012074777,0.0000072181456,0.000027639546,0.000029748586,0.00002179604],"domain_scores_gemma":[0.99956983,0.000055814795,0.00009827354,0.00003485746,0.00016608216,0.000075063625],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026980438,0.00025957418,0.0002858227,0.0012659336,0.00033772434,0.0005587832,0.0003139219,0.00026648727,0.0010627856],"category_scores_gemma":[0.00064158026,0.00016094801,0.00022821166,0.0006032725,0.00020999539,0.00025729527,0.00037923525,0.0001554025,0.00047555595],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013631149,0.00004204834,0.95236945,0.000022163604,0.000046611458,0.00019896915,0.000268863,0.001985473,0.036632072,0.00013005371,0.0001938959,0.007974144],"study_design_scores_gemma":[0.00000708466,0.00008251802,0.9865177,0.000006202512,0.000021743743,0.00013928229,0.0001691049,0.007834622,0.004357585,0.0000867446,0.00076871365,0.000008598664],"about_ca_topic_score_codex":0.002996028,"about_ca_topic_score_gemma":0.004653857,"teacher_disagreement_score":0.002996028,"about_ca_system_score_codex":0.00039356638,"about_ca_system_score_gemma":0.000113779235,"threshold_uncertainty_score":0.005957186},"labels":[],"label_agreement":null},{"id":"W4391777786","doi":"10.3847/1538-4357/ad1591","title":"A Galactic Eclipse: The Small Magellanic Cloud Is Forming Stars in Two Superimposed Systems","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"","keywords":"Physics; Large Magellanic Cloud; Stars; Eclipse; Astrophysics; Astronomy; Small Magellanic Cloud","score_opus":0.016540161266065955,"score_gpt":0.26428662440679357,"score_spread":0.24774646314072762,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391777786","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983217,0.00007664915,0.00034487087,0.00004851729,0.000006729105,0.000006326728,0.0000294768,0.000008441025,0.0011571067],"genre_scores_gemma":[0.99970055,0.000012296612,0.00014501286,0.000011343737,0.000003369577,8.37873e-7,0.00004008891,0.0000013237639,0.00008518447],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980634,0.000034363944,0.000010582675,0.00005577792,0.000040217998,0.00005270422],"domain_scores_gemma":[0.99959177,0.000069662456,0.000091180125,0.000052718497,0.00003918375,0.00015544721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036913328,0.00016983468,0.00028496073,0.00044603148,0.0007786245,0.001011314,0.00043847816,0.00068568374,0.0015148073],"category_scores_gemma":[0.0012241132,0.00016657288,0.00032583973,0.00039009703,0.0006478785,0.0004919066,0.0007556969,0.0002532334,0.00027162916],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006192987,0.00010606659,0.9624155,0.000042637737,0.00008635728,0.001437988,0.0008197657,0.0027931065,0.018539894,0.00412584,0.00040667623,0.008606828],"study_design_scores_gemma":[0.000053301967,0.00017354253,0.9761435,0.000016516053,0.000043161792,0.0009460929,0.0010667397,0.016193377,0.0017653459,0.0020427385,0.0015429718,0.00001267399],"about_ca_topic_score_codex":0.008902372,"about_ca_topic_score_gemma":0.010821189,"teacher_disagreement_score":0.008902372,"about_ca_system_score_codex":0.00083556667,"about_ca_system_score_gemma":0.0003802407,"threshold_uncertainty_score":0.01770109},"labels":[],"label_agreement":null},{"id":"W4391787924","doi":"10.3847/1538-4357/ad0da7","title":"The JWST Advanced Deep Extragalactic Survey: Discovery of an Extreme Galaxy Overdensity at z = 5.4 with JWST/NIRCam in GOODS-S","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":48,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Fondation Merac; University of California, Santa Cruz; Science and Technology Facilities Council; European Commission; Johns Hopkins University; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Research Foundation; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; James Webb Space Telescope; Galaxy; Astronomy; Astrophysics","score_opus":0.013868891703541917,"score_gpt":0.23247003626749166,"score_spread":0.21860114456394975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391787924","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975432,0.00007917251,0.00042392625,0.000042498436,0.0000047405933,0.0000071258655,0.0005171921,0.000044376615,0.0013378378],"genre_scores_gemma":[0.99765956,0.000038623897,0.00084375433,0.00006873206,0.0000111287545,0.000003568036,0.0010411163,0.000012998864,0.00032039994],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997429,0.000019508234,0.000015636744,0.000058033143,0.00009844178,0.00006548799],"domain_scores_gemma":[0.99928844,0.000047242393,0.00021408546,0.000105780055,0.000078360565,0.00026609973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044402937,0.00018013961,0.00018541943,0.0013425025,0.00044613372,0.0005168097,0.00034197967,0.00017843134,0.0012923158],"category_scores_gemma":[0.0004532263,0.0001850577,0.00024295077,0.0006571496,0.00041057038,0.00031361883,0.0010734326,0.00026095586,0.0003657415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012561998,0.00004409571,0.95869815,0.000027072332,0.000069978814,0.00065044465,0.00041083182,0.00013661289,0.028968774,0.0003227368,0.0013298555,0.0092158895],"study_design_scores_gemma":[0.0000040851564,0.000026611782,0.9969694,0.000005838411,0.000013028419,0.000255569,0.000088087,0.000217276,0.000961716,0.000057859175,0.0013976581,0.0000028605393],"about_ca_topic_score_codex":0.0066394205,"about_ca_topic_score_gemma":0.013832776,"teacher_disagreement_score":0.0066394205,"about_ca_system_score_codex":0.00032408469,"about_ca_system_score_gemma":0.00019360485,"threshold_uncertainty_score":0.013201535},"labels":[],"label_agreement":null},{"id":"W4391787953","doi":"10.3847/1538-4357/ad13f4","title":"Constraining the Existence of Axion Clouds in M87* with Closure Trace Analyses","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; TRACE (psycholinguistics); Astrophysics; Axion; Closure (psychology); Astronomy; Dark matter","score_opus":0.024009656431279686,"score_gpt":0.2872197125437871,"score_spread":0.2632100561125074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391787953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9632083,0.000054358552,0.033572588,0.0000666822,0.000007670197,0.000015420768,0.00056647934,0.0004126404,0.0020959207],"genre_scores_gemma":[0.9939861,0.00002229946,0.0050173267,0.000013621042,0.000009768772,0.0000078115745,0.0007680518,0.000054432698,0.00012067235],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979144,0.000045964414,0.000010983632,0.000054062817,0.000044493427,0.000053152875],"domain_scores_gemma":[0.9991217,0.00024013025,0.00022765428,0.00016836869,0.00012629936,0.000115883326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006589222,0.00050962094,0.00031459148,0.0013820376,0.00043618988,0.0013350905,0.0006498713,0.0004190954,0.0013666599],"category_scores_gemma":[0.0019442321,0.00019965258,0.00060022477,0.0008176815,0.00046320213,0.0007858939,0.0011739178,0.0004593195,0.00028870467],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005107357,0.00019721869,0.7020987,0.00011909138,0.00024207933,0.0006712624,0.0004614324,0.14804201,0.05755449,0.021223372,0.0020974362,0.06678216],"study_design_scores_gemma":[0.000044319284,0.00009940363,0.17161109,0.00004294327,0.00008527649,0.00016936258,0.00041869812,0.7902034,0.017453462,0.015209565,0.004613459,0.000049058843],"about_ca_topic_score_codex":0.0057605472,"about_ca_topic_score_gemma":0.004668744,"teacher_disagreement_score":0.0057605472,"about_ca_system_score_codex":0.0005513618,"about_ca_system_score_gemma":0.00047066578,"threshold_uncertainty_score":0.011454046},"labels":[],"label_agreement":null},{"id":"W4391825225","doi":"10.3847/1538-4357/ad165b","title":"Filamentary Network and Magnetic Field Structures Revealed with BISTRO in the High-mass Star-forming Region NGC 2264: Global Properties and Local Magnetogravitational Configurations","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Western University; University of Manitoba; McMaster University; Queen's University; Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Engineering Research Board; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Ministry of Science and ICT, South Korea; Agencia Canaria de Investigación, Innovación y Sociedad de la Información; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; Academia Sinica; National Natural Science Foundation of China; Department of Science and Technology, Ministry of Science and Technology, India; Science and Technology Facilities Council; National Research Foundation; National Astronomical Research Institute of Thailand; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Protein filament; Magnetic field; Gravitation; Polarization (electrochemistry); Perpendicular; Astronomy; Geometry","score_opus":0.009789846708437612,"score_gpt":0.21728085065416594,"score_spread":0.20749100394572834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391825225","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998896,0.000028458593,0.00042497285,0.000007850018,7.0540557e-7,0.0000023453051,0.00015325496,0.0000285117,0.0004579087],"genre_scores_gemma":[0.9994312,0.000012363064,0.0003197124,0.000002359224,0.0000026271548,0.0000020371344,0.00014417124,0.0000033366796,0.000082109866],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995244,0.0000053752265,0.0000029131743,0.000015408663,0.000009673064,0.0000142171275],"domain_scores_gemma":[0.9997099,0.000037151356,0.000117413816,0.00003571932,0.00003757989,0.00006227694],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000085691216,0.00013969654,0.00013811112,0.0012288194,0.0002212054,0.00032515518,0.00019075896,0.00013558916,0.00074626715],"category_scores_gemma":[0.00029714996,0.00011952606,0.00012146692,0.00043765744,0.00019739871,0.00015115777,0.00023990018,0.00010132511,0.00013652703],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025451995,0.000053051044,0.7469499,0.000033675755,0.000086501714,0.00039263035,0.00026831747,0.0020048337,0.23913422,0.00019825721,0.00020947604,0.010414683],"study_design_scores_gemma":[0.00000263116,0.000022367738,0.9942694,0.0000017908351,0.000013512603,0.00011701764,0.00007423871,0.0020814538,0.0032449665,0.000055212895,0.00011335089,0.000004159094],"about_ca_topic_score_codex":0.0021207207,"about_ca_topic_score_gemma":0.002357106,"teacher_disagreement_score":0.0021207207,"about_ca_system_score_codex":0.00016903496,"about_ca_system_score_gemma":0.00006124149,"threshold_uncertainty_score":0.00421679},"labels":[],"label_agreement":null},{"id":"W4391871452","doi":"10.3847/1538-4357/ad2994","title":"A 350 MHz Green Bank Telescope Survey of Unassociated Fermi LAT Sources: Discovery and Timing of 10 Millisecond Pulsars","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Istituto Nazionale di Astrofisica; National Science Foundation; Agenzia Spaziale Italiana; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Precursory Research for Embryonic Science and Technology; York University; Japan Society for the Promotion of Science; Canadian Institute for Advanced Research; New York University Abu Dhabi; Office of Naval Research; Centre National de la Recherche Scientifique; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Japan Aerospace Exploration Agency; U.S. Department of Energy; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet","keywords":"Physics; Pulsar; Millisecond pulsar; Fermi Gamma-ray Space Telescope; Astrophysics; Green Bank Telescope; Telescope; Astronomy; Radio telescope; Sky; Gamma ray","score_opus":0.02700943747609114,"score_gpt":0.31983942235709045,"score_spread":0.2928299848809993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391871452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966444,0.00038393712,0.00017595783,0.00006512093,0.000003691498,0.0000064492588,0.0015287722,0.000026453738,0.0011653291],"genre_scores_gemma":[0.996345,0.00030122805,0.00054712384,0.000095720905,0.000019348836,0.000012648247,0.0018371878,0.000011258836,0.00083063066],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981946,0.000028734277,0.000016466156,0.000040905597,0.00004325134,0.00005117566],"domain_scores_gemma":[0.9991171,0.00013266313,0.0003673904,0.000068593356,0.00011698295,0.00019729102],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003837318,0.00020433559,0.00019845783,0.0027979931,0.00047681187,0.0005513542,0.0002983385,0.00019681406,0.0020232247],"category_scores_gemma":[0.0005733947,0.00017588102,0.00008796146,0.0016011,0.00020412469,0.0003511342,0.0005995821,0.00018266367,0.00070983573],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010910234,0.000031871085,0.9786982,0.00001873533,0.000019200601,0.00019878024,0.0003835503,0.00004758698,0.006201075,0.000117152464,0.0010671956,0.013107723],"study_design_scores_gemma":[0.000004634378,0.00003070459,0.9975783,0.000010221445,0.000008100478,0.00020658552,0.00010722454,0.00011574978,0.0005768597,0.000023072242,0.0013347155,0.0000036799202],"about_ca_topic_score_codex":0.013288985,"about_ca_topic_score_gemma":0.024838978,"teacher_disagreement_score":0.013288985,"about_ca_system_score_codex":0.00044015792,"about_ca_system_score_gemma":0.00030060575,"threshold_uncertainty_score":0.026423275},"labels":[],"label_agreement":null},{"id":"W4391886799","doi":"10.3847/1538-4357/ad19d0","title":"A Physically Motivated Framework to Compare Pair Fractions of Isolated Low- and High-mass Galaxies across Cosmic Time","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Trent University","funders":"National Aeronautics and Space Administration; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; COSMIC cancer database; Galaxy; Astrophysics; Astronomy","score_opus":0.005701154649599584,"score_gpt":0.23212798235757806,"score_spread":0.22642682770797848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391886799","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9606463,0.00010236914,0.033697467,0.0002522553,0.000019781466,0.0000336291,0.00064963853,0.00026462792,0.0043339226],"genre_scores_gemma":[0.99459803,0.0000181937,0.0047229026,0.00004197959,0.000006473437,0.000025639103,0.00026830513,0.000030742405,0.0002876219],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99975353,0.00008771038,0.000008064804,0.00008667926,0.000030226249,0.00003364831],"domain_scores_gemma":[0.9990268,0.00035975437,0.0002278846,0.0001829242,0.000051087023,0.00015159309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009970004,0.000247782,0.0003474662,0.0010474918,0.0006587034,0.0011810327,0.0011795003,0.00069432834,0.002787538],"category_scores_gemma":[0.004451986,0.00023347263,0.0005141581,0.0005875741,0.0011900748,0.0010809395,0.0011194897,0.0007819251,0.00020693899],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031914492,0.00024506074,0.26729336,0.00008076353,0.00028394704,0.00036334147,0.00033351532,0.5990875,0.011186058,0.10553719,0.0018579414,0.013412223],"study_design_scores_gemma":[0.00008709143,0.00012217503,0.08491232,0.000012172082,0.000047236772,0.00014155626,0.00012423021,0.87529093,0.0023609705,0.035178564,0.0016810729,0.000041632986],"about_ca_topic_score_codex":0.0037265914,"about_ca_topic_score_gemma":0.002736061,"teacher_disagreement_score":0.0037265914,"about_ca_system_score_codex":0.0007324981,"about_ca_system_score_gemma":0.00030521824,"threshold_uncertainty_score":0.009325206},"labels":[],"label_agreement":null},{"id":"W4391886809","doi":"10.3847/1538-4357/ad16e8","title":"Orbital Torus Imaging: Acceleration, Density, and Dark Matter in the Galactic Disk Measured with Element Abundance Gradients","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Astrophysics; Torus; Astronomy; Acceleration; Dark matter; Abundance (ecology); Classical mechanics","score_opus":0.009601401142339143,"score_gpt":0.22438669613222859,"score_spread":0.21478529498988944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391886809","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913629,0.000063834,0.0033967325,0.000048365597,0.000003899098,0.0000059787044,0.0015026522,0.00029880772,0.0033168797],"genre_scores_gemma":[0.9963026,0.000024276456,0.002756762,0.000010530273,0.0000056230265,0.000002296064,0.000606553,0.000024634732,0.00026678026],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999528,0.00000830458,0.0000032713501,0.000013351367,0.000014698021,0.000007675202],"domain_scores_gemma":[0.9997768,0.00006627583,0.00006837137,0.000026072075,0.000031531934,0.000030903007],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014651132,0.0001063611,0.00008309729,0.0010447492,0.0000917004,0.00039470522,0.000101019774,0.00009386935,0.0024152293],"category_scores_gemma":[0.0005995947,0.0000726724,0.000047730962,0.0007512784,0.0001362361,0.0003501901,0.00023486424,0.00006088488,0.00040940137],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023333625,0.000037446014,0.9107983,0.00003407282,0.000035196466,0.000108618486,0.00023013708,0.0028844387,0.041343138,0.0010674276,0.002815754,0.040412053],"study_design_scores_gemma":[0.000008991582,0.000033977103,0.96386206,0.000008701627,0.000012722182,0.00022402126,0.00016996365,0.020197859,0.013450015,0.00064558286,0.0013770096,0.000009153242],"about_ca_topic_score_codex":0.0028307766,"about_ca_topic_score_gemma":0.0035962006,"teacher_disagreement_score":0.0028307766,"about_ca_system_score_codex":0.00014538725,"about_ca_system_score_gemma":0.000055074514,"threshold_uncertainty_score":0.008079767},"labels":[],"label_agreement":null},{"id":"W4391886837","doi":"10.3847/1538-4357/ad11f0","title":"The Green Bank North Celestial Cap Survey. IX. Timing Follow-up for 128 Pulsars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Canadian Institute for Advanced Research; Horizon 2020 Framework Programme; Office of Naval Research; Alliance de recherche numérique du Canada; University of Toronto; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Foundation; University of Central Florida; Smithsonian Astrophysical Observatory; McGill University; National Aeronautics and Space Administration","keywords":"Physics; Pulsar; Astronomy; Astrophysics","score_opus":0.028922750208883043,"score_gpt":0.3318840427435148,"score_spread":0.3029612925346318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391886837","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8291913,0.0015107587,0.0008161727,0.00054760894,0.00013817119,0.00028051028,0.14632602,0.0004525182,0.020736849],"genre_scores_gemma":[0.80137604,0.0012326731,0.004836576,0.00047417797,0.00013402665,0.00031350608,0.17063114,0.000207171,0.020794746],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99947566,0.000037750375,0.00004041351,0.000109542096,0.00020119688,0.00013543475],"domain_scores_gemma":[0.99743325,0.00012214514,0.00044812527,0.00031939812,0.0011201503,0.0005569132],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007228919,0.00030089734,0.0003547896,0.0041612047,0.0013527805,0.0007800828,0.0005945681,0.00029952836,0.0040339106],"category_scores_gemma":[0.0014765398,0.00026129917,0.00017687208,0.005175572,0.00027085954,0.00030145267,0.0007873598,0.00038519123,0.0022334557],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027991718,0.000062140345,0.92501485,0.0000767625,0.000034740424,0.00052015804,0.00069356256,0.00018493987,0.0029643155,0.0001390756,0.029735006,0.040294588],"study_design_scores_gemma":[0.000013306613,0.000013859602,0.9891265,0.000010998669,0.00000650741,0.0000620506,0.000098418255,0.000118948876,0.0002302232,0.000013962324,0.010298881,0.000006216341],"about_ca_topic_score_codex":0.6692188,"about_ca_topic_score_gemma":0.81862986,"teacher_disagreement_score":0.6692188,"about_ca_system_score_codex":0.0025875312,"about_ca_system_score_gemma":0.0036311478,"threshold_uncertainty_score":0.6654585},"labels":[],"label_agreement":null},{"id":"W4391934301","doi":"10.3847/1538-4357/ad17b8","title":"A Robust Study of High-redshift Galaxies: Unsupervised Machine Learning for Characterizing Morphology with JWST up to z ∼ 8","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Astronomy; James Webb Space Telescope; Galaxy; Redshift; Galaxy formation and evolution; Star formation; Galaxy merger; COSMIC cancer database; Luminous infrared galaxy","score_opus":0.014666268811080522,"score_gpt":0.22389585676883178,"score_spread":0.20922958795775126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391934301","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9837937,0.000057488513,0.015226963,0.00006443844,0.000004003194,0.0000083312625,0.00031569088,0.00015426052,0.0003751642],"genre_scores_gemma":[0.9941162,0.000015274572,0.0050058276,0.000007914117,0.0000057193834,0.0000041842072,0.00068686303,0.000012862896,0.00014512136],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99982375,0.00003489103,0.000009676211,0.000054104432,0.000043657983,0.000033983106],"domain_scores_gemma":[0.9991385,0.00026040713,0.00020380651,0.00017046853,0.00014318152,0.00008369812],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007705835,0.00025858713,0.00019783965,0.001066738,0.00019896125,0.00057753467,0.00046774917,0.000317652,0.00031702846],"category_scores_gemma":[0.0023314585,0.00015742154,0.00031515854,0.00055461837,0.0003378575,0.00046821937,0.00046545969,0.0004154797,0.000144056],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021511615,0.00017883949,0.6622713,0.00006149414,0.00023894879,0.00019872372,0.00020594137,0.17288983,0.041495614,0.00245794,0.0014279052,0.118358344],"study_design_scores_gemma":[0.0000064440064,0.00004530257,0.26557472,0.000008230071,0.000015693568,0.000045769582,0.0000476636,0.7275933,0.005326842,0.00092359015,0.00040382947,0.0000086143955],"about_ca_topic_score_codex":0.007196622,"about_ca_topic_score_gemma":0.008379906,"teacher_disagreement_score":0.007196622,"about_ca_system_score_codex":0.00036767664,"about_ca_system_score_gemma":0.00029027983,"threshold_uncertainty_score":0.014309466},"labels":[],"label_agreement":null},{"id":"W4391995315","doi":"10.3847/1538-4357/ad1101","title":"“Beads-on-a-string” Star Formation Tied to One of the Most Powerful Active Galactic Nucleus Outbursts Observed in a Cool-core Galaxy Cluster","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Science and Technology Facilities Council; Agencia Nacional de Investigación y Desarrollo; National Institutes of Natural Sciences; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Astronomical Observatory of Japan; National Radio Astronomy Observatory; Universitetet i Oslo; Natural Sciences and Engineering Research Council of Canada; National Science Council; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Stockholms Universitet; Turun Yliopisto; Space Telescope Science Institute; ASTRON; Háskóli Íslands; Aarhus Universitet; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Galaxy; Intracluster medium; Active galactic nucleus; Redshift; Stars; Astronomy; Globular cluster; Galaxy cluster","score_opus":0.018548760148514327,"score_gpt":0.2329125177018162,"score_spread":0.21436375755330186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4391995315","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99931717,0.0000139790445,0.000066402354,0.000034242603,0.0000029386463,0.0000020330497,0.00005594765,0.000012187159,0.0004950492],"genre_scores_gemma":[0.99967897,0.0000053775857,0.000050724197,0.000020541469,0.000004122281,9.272546e-7,0.000068961155,0.0000013697531,0.00016900538],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992204,0.000006445175,0.0000047262993,0.000032946766,0.000010205808,0.000023543387],"domain_scores_gemma":[0.99949014,0.000025584268,0.00015585769,0.00006500679,0.000032537435,0.00023083315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008788441,0.00012588946,0.00014532128,0.00034390896,0.00055642263,0.0003816121,0.00022811462,0.00023545393,0.0019875017],"category_scores_gemma":[0.0003314685,0.000095733616,0.00013691722,0.00022065033,0.00044964728,0.00016614569,0.00042189268,0.0002565501,0.00024774656],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018949085,0.000060444894,0.97736347,0.000008141312,0.00003943854,0.00042115164,0.00015317948,0.00018112668,0.017947966,0.00020548608,0.0004773258,0.0029528344],"study_design_scores_gemma":[0.0000022636566,0.000032936376,0.99853384,0.000001048655,0.0000075246253,0.00019385215,0.00007793783,0.00027508655,0.00063528464,0.00005437016,0.00018368226,0.0000021785138],"about_ca_topic_score_codex":0.0034592082,"about_ca_topic_score_gemma":0.0073589645,"teacher_disagreement_score":0.0034592082,"about_ca_system_score_codex":0.00023295965,"about_ca_system_score_gemma":0.000110646826,"threshold_uncertainty_score":0.0068781376},"labels":[],"label_agreement":null},{"id":"W4392019335","doi":"10.3847/1538-4357/ad5a7e","title":"The Santa Barbara Binary−disk Code Comparison","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"HORIZON EUROPE Marie Sklodowska-Curie Actions; HORIZON EUROPE European Research Council; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Graduate School, University of Maryland; Horizon 2020 Framework Programme; Deutsche Forschungsgemeinschaft; Nuclear Safety and Security Commission; European Commission; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Binary number; Binary Independence Model; Astrophysics; Binary code; Eccentricity (behavior); Machine epsilon; Torque; Computational physics; Statistical physics; Algorithm; Thermodynamics; Mathematics","score_opus":0.014504495450726688,"score_gpt":0.2800087720202923,"score_spread":0.2655042765695656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392019335","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94786197,0.00033326412,0.008744191,0.00038430805,0.00011558817,0.00014193013,0.0049303886,0.0073873075,0.030101063],"genre_scores_gemma":[0.93850255,0.00013474115,0.049121678,0.00015125462,0.000023835973,0.0002344215,0.006954496,0.001556813,0.0033201748],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99898773,0.00023651548,0.00010960395,0.00019584724,0.0003327333,0.00013758878],"domain_scores_gemma":[0.99586725,0.0012724955,0.00019188719,0.00095505686,0.0015166048,0.00019681045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013010764,0.0006963601,0.00079575303,0.0010812357,0.0010991027,0.00149937,0.0018973101,0.00083440146,0.005544798],"category_scores_gemma":[0.0059567303,0.00036016043,0.00050896924,0.001433455,0.00055439566,0.000818532,0.0008994841,0.00071827136,0.0012717405],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0031664467,0.001430274,0.07140167,0.0008831976,0.00063990307,0.00045730214,0.0011476014,0.6717467,0.01881378,0.029552974,0.047698643,0.15306155],"study_design_scores_gemma":[0.0003703841,0.0002132122,0.013247949,0.000049842085,0.000050823528,0.00005913787,0.0002455448,0.96056014,0.011238581,0.002132238,0.011758661,0.000073584095],"about_ca_topic_score_codex":0.030138252,"about_ca_topic_score_gemma":0.03392314,"teacher_disagreement_score":0.030138252,"about_ca_system_score_codex":0.001868527,"about_ca_system_score_gemma":0.0013358244,"threshold_uncertainty_score":0.059925675},"labels":[],"label_agreement":null},{"id":"W4392019584","doi":"10.3847/1538-4357/ad3ba8","title":"The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Astrophysics; Redshift; Binary number; Mass distribution; Star (game theory); Physics; Distribution (mathematics); Binary black hole; Astronomy; Mathematics; Galaxy","score_opus":0.010123462400119151,"score_gpt":0.22528095670472234,"score_spread":0.21515749430460318,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392019584","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990396,0.000028258399,0.00031371735,0.000010034207,7.118294e-7,0.0000014358109,0.00022789014,0.000024020084,0.00035434007],"genre_scores_gemma":[0.99930894,0.000017790182,0.0001159893,0.0000019311067,0.000001574959,6.791991e-7,0.00047008268,0.0000042573965,0.00007877947],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988985,0.000016367268,0.0000037773389,0.000034179007,0.000028464856,0.000027310238],"domain_scores_gemma":[0.9990075,0.0002986749,0.0003342487,0.00010887727,0.00012748117,0.00012324392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043853943,0.00023434755,0.00018142934,0.0013944979,0.00019705082,0.0006014085,0.0002834366,0.0002752749,0.0010701861],"category_scores_gemma":[0.0015792,0.00020914695,0.0002022372,0.00059025537,0.00024690593,0.00032300447,0.00041850636,0.00015751811,0.0001818521],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026123523,0.000031296535,0.92670953,0.000030293893,0.00009071572,0.00015819156,0.00024036024,0.040837713,0.021186534,0.0023316275,0.00045840917,0.007664063],"study_design_scores_gemma":[0.000014407807,0.000043747717,0.9465599,0.0000040460195,0.000020059348,0.00006685008,0.00006242795,0.049045153,0.0029634826,0.00086056016,0.00034574978,0.000013725256],"about_ca_topic_score_codex":0.0048041344,"about_ca_topic_score_gemma":0.0033897173,"teacher_disagreement_score":0.0048041344,"about_ca_system_score_codex":0.00042514858,"about_ca_system_score_gemma":0.00009462562,"threshold_uncertainty_score":0.00955236},"labels":[],"label_agreement":null},{"id":"W4392035942","doi":"10.3847/1538-4357/ad1ce4","title":"Detection of X-Ray Polarization from the Blazar 1ES 1959+650 with the Imaging X-Ray Polarimetry Explorer","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Istituto Nazionale di Fisica Nucleare; Ministerio de Ciencia e Innovación; Agencia Estatal de Investigación; Goddard Space Flight Center; University of Crete; National Science Foundation; Agenzia Spaziale Italiana; Nuclear Safety and Security Commission; California Institute of Technology; National Aeronautics and Space Administration; Oak Ridge Associated Universities; Instituto de Astrofísica de Andalucía; Marshall Space Flight Center; Istituto Nazionale di Astrofisica","keywords":"Physics; Blazar; Polarimetry; X-ray; Polarization (electrochemistry); Astronomy; Astrophysics; X-ray astronomy; X-ray telescope; Quasar; Gamma ray; Optics; Scattering; Galaxy; Telescope","score_opus":0.005390071789266301,"score_gpt":0.2001716325440521,"score_spread":0.1947815607547858,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392035942","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9949222,0.00015978579,0.00080134376,0.000052499552,0.000008299272,0.000012379436,0.0006297838,0.00005449103,0.003359193],"genre_scores_gemma":[0.9980002,0.00006257403,0.00071198016,0.00003205434,0.000011706326,0.000004562495,0.00079148146,0.00000941056,0.000376093],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998945,0.00001084106,0.00000498332,0.00003345147,0.00003251839,0.000023667699],"domain_scores_gemma":[0.99978834,0.000018522462,0.00009249854,0.000024568857,0.000024400268,0.000051645075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002785465,0.00025560596,0.00012287068,0.0009097332,0.00029032218,0.0005909089,0.00015841945,0.00023380901,0.001105603],"category_scores_gemma":[0.00028633492,0.00016964159,0.00015282238,0.0005683175,0.00021979155,0.00021931781,0.0003666787,0.00029429814,0.00023024248],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004759928,0.00010723047,0.6849439,0.000078669815,0.00014767227,0.0009402524,0.00053622347,0.00070063357,0.2917742,0.00084318686,0.0012073397,0.018244803],"study_design_scores_gemma":[0.000014126849,0.000054016135,0.9907093,0.000008365245,0.000023925368,0.00019050852,0.00005762625,0.000456409,0.007043494,0.00005843629,0.0013778089,0.00000607911],"about_ca_topic_score_codex":0.0027618115,"about_ca_topic_score_gemma":0.0050904807,"teacher_disagreement_score":0.0027618115,"about_ca_system_score_codex":0.00027869022,"about_ca_system_score_gemma":0.00012090278,"threshold_uncertainty_score":0.0054915547},"labels":[],"label_agreement":null},{"id":"W4392104485","doi":"10.3847/1538-4357/ad0f1d","title":"A Detection of Cosmological 21 cm Emission from CHIME in Cross-correlation with eBOSS Measurements of the Lyα Forest","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Fonds de recherche du Québec – Nature et technologies; Office of Science; National Research Council Canada; University of Toronto; Canada Research Chairs; Alliance de recherche numérique du Canada; Industry Canada; Canada Foundation for Innovation; University of Utah; Smithsonian Astrophysical Observatory; Western Canada Research Grid; Canadian Institute for Advanced Research; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Alfred P. Sloan Foundation; McGill University; U.S. Department of Energy; Government of Canada; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy","score_opus":0.01383406940020175,"score_gpt":0.2381986290209824,"score_spread":0.22436455962078067,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392104485","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99524975,0.00013476002,0.0010914047,0.000051727795,0.0000069161333,0.000010276548,0.0005948296,0.00010457875,0.0027557088],"genre_scores_gemma":[0.9983436,0.000030646195,0.0005886237,0.000030778352,0.0000045645306,0.0000042178185,0.0005595835,0.000012109315,0.00042591654],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965405,0.000018582641,0.0000060400553,0.00010222148,0.00012606572,0.00009303618],"domain_scores_gemma":[0.9993656,0.00008669886,0.00013531423,0.000088990484,0.00014826198,0.00017501847],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042016208,0.00025992683,0.0002054752,0.0008556259,0.000491511,0.000434353,0.0002375141,0.00025447062,0.0013923873],"category_scores_gemma":[0.0008343617,0.0002133055,0.00016332947,0.0006415546,0.00040671654,0.00014098173,0.0006068838,0.00031583654,0.00022723264],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042093248,0.000053430653,0.84821963,0.00003257074,0.00012921757,0.0006836049,0.0005439731,0.00040580603,0.1327525,0.00024361728,0.0012341108,0.015280485],"study_design_scores_gemma":[0.0000017592115,0.000008998701,0.9963398,0.0000015428534,0.000009691272,0.00012060402,0.000034014483,0.00016499037,0.0026985025,0.000017205955,0.0005985562,0.000004439984],"about_ca_topic_score_codex":0.062394723,"about_ca_topic_score_gemma":0.16259448,"teacher_disagreement_score":0.062394723,"about_ca_system_score_codex":0.0006331408,"about_ca_system_score_gemma":0.0003649559,"threshold_uncertainty_score":0.124063134},"labels":[],"label_agreement":null},{"id":"W4392104993","doi":"10.3847/1538-4357/ad2168","title":"Measuring the Mass–Radius Relation of White Dwarfs Using Wide Binaries","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Leibniz-Gemeinschaft; University of Colorado Boulder; National Astronomical Observatories, Chinese Academy of Sciences; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; Leibniz-Institut für Astrophysik Potsdam; New Mexico State University; Nanjing University; Yale University; University of Toronto; École Polytechnique Fédérale de Lausanne; Space Telescope Science Institute; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Harvard University; China National Textile and Apparel Council; National Science Foundation; Yunnan University; California Institute of Technology; Ohio State University; Smithsonian Astrophysical Observatory; Flatiron Health; Smithsonian Institution","keywords":"White dwarf; Physics; Astrophysics; Gravitational redshift; RADIUS; Redshift; Astronomy; Black dwarf; Gravitation; Stars; Galaxy","score_opus":0.02325467387396458,"score_gpt":0.2286288015760218,"score_spread":0.20537412770205724,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392104993","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9929052,0.00025148,0.004935792,0.000013917341,0.0000051493225,0.0000058968685,0.00024383137,0.000103607184,0.001535173],"genre_scores_gemma":[0.9979087,0.000033244036,0.0016969023,0.000008595878,0.0000043211744,0.00000209655,0.00022287646,0.000010083046,0.000113248796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997402,0.00003079737,0.000015527417,0.00012354375,0.00006116705,0.000028791519],"domain_scores_gemma":[0.9992741,0.00015351782,0.00022081869,0.00011216467,0.00010092833,0.00013848323],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006585612,0.00023178452,0.0003232531,0.0016243057,0.00040499482,0.00068568997,0.00025835127,0.00016075384,0.0004972346],"category_scores_gemma":[0.0012581911,0.0001466002,0.00014621447,0.0009554993,0.00027974782,0.00058639894,0.0009324578,0.00017687766,0.00030740997],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008301579,0.000031250405,0.94703287,0.000024218925,0.00012320647,0.000055464643,0.0002888423,0.0019578664,0.03249572,0.0009964603,0.00021719097,0.016693737],"study_design_scores_gemma":[0.0000027364667,0.000041328578,0.9858914,0.000004742352,0.000017253653,0.00010755843,0.000100186284,0.00517715,0.0072690416,0.00061589,0.00076509046,0.000007614065],"about_ca_topic_score_codex":0.0036595543,"about_ca_topic_score_gemma":0.007088252,"teacher_disagreement_score":0.0036595543,"about_ca_system_score_codex":0.00033649086,"about_ca_system_score_gemma":0.0001216176,"threshold_uncertainty_score":0.0072764754},"labels":[],"label_agreement":null},{"id":"W4392191614","doi":"10.3847/1538-4357/ad1e5b","title":"Zero Metallicity with Zero CPU Hours: Masses of the First Stars on the Laptop","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"History and Developments in Astronomy","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Korea Institute for Advanced Study; Royal Society; Astrophysics Division; Government of Canada","keywords":"Physics; Zero (linguistics); Laptop; Metallicity; Stars; Astrophysics; Astronomy; Zero-point energy; Operating system; Quantum mechanics","score_opus":0.01034110573254355,"score_gpt":0.2159482233532832,"score_spread":0.20560711762073966,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392191614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5697718,0.00044040493,0.3869161,0.0015716996,0.000071895636,0.000082952785,0.00083772466,0.0011720065,0.039135404],"genre_scores_gemma":[0.965934,0.0002606385,0.022548707,0.00011839462,0.000041124007,0.000090357324,0.00020910283,0.000189265,0.0106085455],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998872,0.000023698312,0.000002768615,0.000027182845,0.000021526708,0.000037537407],"domain_scores_gemma":[0.9995931,0.00015163969,0.000068383524,0.00005547508,0.000057349593,0.000074140116],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003432262,0.0006022034,0.000490983,0.0004655593,0.00055774505,0.0014422573,0.0014379313,0.00075130886,0.0049609807],"category_scores_gemma":[0.002337234,0.00035933766,0.0005425417,0.0003362026,0.0009596674,0.0014212446,0.00066277036,0.00071997265,0.0010713546],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000077970566,0.000039695384,0.0053765564,0.00003661251,0.000015798603,0.00023723608,0.00012443001,0.90756965,0.002287788,0.07767199,0.0011284549,0.0054338407],"study_design_scores_gemma":[0.000012738453,0.00001049809,0.00046710228,0.0000062820063,0.000005101797,0.0000491904,0.000016511909,0.9887628,0.00039209292,0.009687999,0.0005837033,0.000005939521],"about_ca_topic_score_codex":0.014491958,"about_ca_topic_score_gemma":0.0067729033,"teacher_disagreement_score":0.014491958,"about_ca_system_score_codex":0.0010685144,"about_ca_system_score_gemma":0.0010694417,"threshold_uncertainty_score":0.02881521},"labels":[],"label_agreement":null},{"id":"W4392191797","doi":"10.3847/1538-4357/ad1e54","title":"Tidal Migration of Exoplanets around M Dwarfs: Frequency-dependent Tidal Dissipation","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Exoplanet; Planet; Dissipation; Astrophysics; Tidal acceleration; Planetary system; Dissipative system; Hot Jupiter; Tidal heating; Astronomy; Orb (optics); Orbital decay","score_opus":0.011255389386908381,"score_gpt":0.2373923033012567,"score_spread":0.22613691391434834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392191797","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99895275,0.00001272233,0.0005602999,0.000016415677,0.0000014502922,0.00000128023,0.000027206926,0.000020409156,0.00040741716],"genre_scores_gemma":[0.99965835,0.000006990298,0.00018300947,0.000002770271,8.545474e-7,9.0481154e-7,0.000027364289,0.0000055660767,0.000114246446],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99997115,0.00000649265,0.0000022078839,0.0000080075415,0.000005057817,0.000007112484],"domain_scores_gemma":[0.9998271,0.00005286908,0.000040487565,0.000021741504,0.000023789451,0.0000339897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014884559,0.00020421286,0.0001694846,0.0002978156,0.00032694626,0.00035186688,0.00028390475,0.00027250277,0.00060674764],"category_scores_gemma":[0.0007467901,0.00013892396,0.00024305157,0.00023641041,0.00029648325,0.0002839551,0.00027695578,0.00018010767,0.00006609121],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026331312,0.00010431039,0.19955325,0.00004135402,0.00008056309,0.0005140136,0.0002991905,0.7628333,0.027020823,0.0027301032,0.00031311566,0.006246689],"study_design_scores_gemma":[0.000027769524,0.000058966976,0.06380563,0.0000050335043,0.000010192072,0.00007340462,0.0000823997,0.9324084,0.0026761563,0.0006309781,0.00020903772,0.000012011362],"about_ca_topic_score_codex":0.007718709,"about_ca_topic_score_gemma":0.0046662344,"teacher_disagreement_score":0.007718709,"about_ca_system_score_codex":0.00046506475,"about_ca_system_score_gemma":0.00020588486,"threshold_uncertainty_score":0.01534754},"labels":[],"label_agreement":null},{"id":"W4392199313","doi":"10.3847/1538-4357/ad1600","title":"Global Chemical Transport on Hot Jupiters: Insights from the 2D VULCAN Photochemical Model","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; Indian Council of Agricultural Research; National Aeronautics and Space Administration","keywords":"Hot Jupiter; Physics; Exoplanet; Astrophysics; Atmospheric sciences; Atmospheric circulation; Planet","score_opus":0.011443947658521978,"score_gpt":0.22678511924885328,"score_spread":0.2153411715903313,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392199313","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9733166,0.00047073243,0.008272025,0.00090372947,0.000052127143,0.000036897996,0.0022083246,0.000266398,0.014473123],"genre_scores_gemma":[0.9957119,0.00020535695,0.0016188244,0.00009874393,0.000026781385,0.00003057398,0.0007454073,0.000049397375,0.0015128719],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999217,0.00001984157,0.0000029960174,0.000022517046,0.000012161908,0.000020817459],"domain_scores_gemma":[0.9997888,0.00007477102,0.00003650762,0.000019815732,0.00003354895,0.0000466245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020268177,0.0006465631,0.00041039486,0.0004197515,0.00079636555,0.0012285752,0.0011622327,0.0012946954,0.0018026291],"category_scores_gemma":[0.00067678775,0.00031062175,0.0006359563,0.00047016918,0.0006442088,0.00064717646,0.00085054495,0.00077476987,0.0001292286],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004245127,0.0000369245,0.00499217,0.000019615765,0.000028327146,0.000097004886,0.00003543555,0.98947316,0.0010679142,0.0027762025,0.00052558404,0.0009051423],"study_design_scores_gemma":[0.000019117339,0.00000833038,0.0013602591,0.0000023239518,0.00000729866,0.000008464034,0.000018945877,0.9976273,0.00010690756,0.00053150125,0.00030219075,0.0000073941865],"about_ca_topic_score_codex":0.19264205,"about_ca_topic_score_gemma":0.056709714,"teacher_disagreement_score":0.19264205,"about_ca_system_score_codex":0.0018531758,"about_ca_system_score_gemma":0.0010357946,"threshold_uncertainty_score":0.38304144},"labels":[],"label_agreement":null},{"id":"W4392238079","doi":"10.3847/1538-4357/ad0726","title":"The NANOGrav 12.5 yr Data Set: Search for Gravitational Wave Memory","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Office of Naval Research; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Jet Propulsion Laboratory; Council for Higher Education; College of Science, Oregon State University; California Institute of Technology; Israel Academy of Sciences and Humanities; Alfred P. Sloan Foundation; Brinson Foundation; Goddard Space Flight Center; National Radio Astronomy Observatory; Space Telescope Science Institute; Oregon State University; Canadian Institute for Advanced Research; Research Corporation for Science Advancement; Vanderbilt University; University of Toronto; Associated Universities; Texas Tech University; Gordon and Betty Moore Foundation; Flatiron Health; Eötvös Loránd Tudományegyetem; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; University of Central Florida; National Science Foundation","keywords":"Physics; Pulsar; Astrophysics; Sky; Gravitational wave; Noise (video); Amplitude; Epoch (astronomy); Astronomy; Stars; Artificial intelligence; Quantum mechanics; Computer science","score_opus":0.05427092982925991,"score_gpt":0.3747442531743488,"score_spread":0.3204733233450889,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392238079","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97451967,0.00030254415,0.004596156,0.0004958604,0.000030704734,0.000031024098,0.016586117,0.00021461144,0.0032233312],"genre_scores_gemma":[0.9419062,0.00008675408,0.005418747,0.00019843517,0.00003518283,0.000045909386,0.05099438,0.000110388304,0.0012039897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9989039,0.00036363886,0.00006496941,0.00024632987,0.00033946225,0.00008169244],"domain_scores_gemma":[0.9946936,0.0028346232,0.00082097395,0.0008315997,0.0004889256,0.000330325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0031191066,0.00033670955,0.00071422604,0.0019507878,0.0006789109,0.0009983644,0.00087372935,0.000705801,0.0031709988],"category_scores_gemma":[0.008959014,0.00022174217,0.0005598027,0.0017324975,0.00046696715,0.0007282211,0.0009979212,0.0007036297,0.0009543951],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023247225,0.00051183,0.82801896,0.00037330258,0.0010636917,0.0009750447,0.0005079471,0.04514779,0.024741927,0.0054252306,0.03071593,0.06019355],"study_design_scores_gemma":[0.00039203942,0.0004652215,0.80182827,0.00011334731,0.00029962513,0.0008922878,0.0007439211,0.14344166,0.00863593,0.0046831546,0.038373053,0.00013144067],"about_ca_topic_score_codex":0.009600516,"about_ca_topic_score_gemma":0.015721977,"teacher_disagreement_score":0.009600516,"about_ca_system_score_codex":0.0004645548,"about_ca_system_score_gemma":0.0005258346,"threshold_uncertainty_score":0.019089282},"labels":[],"label_agreement":null},{"id":"W4392294001","doi":"10.3847/1538-4357/ad1835","title":"Submillimeter-wavelength Polarimetry of IRC+10216","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Science and Technology Facilities Council; National Astronomical Observatory of Japan; Academia Sinica; National Aeronautics and Space Administration; National Science Foundation; Korea Astronomy and Space Science Institute; Universities Space Research Association","keywords":"Physics; Polarimetry; Astronomy; Wavelength; Astrophysics; Millimeter; Astrobiology; Optics; Scattering","score_opus":0.010909857810707196,"score_gpt":0.24435971646121551,"score_spread":0.23344985865050832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392294001","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936487,0.00008464853,0.00025159612,0.000034405955,0.000009735624,0.000012507145,0.00124651,0.00006871443,0.004643168],"genre_scores_gemma":[0.9953506,0.000045588717,0.001256861,0.000055853907,0.000020267064,0.000014582207,0.002660247,0.00002661668,0.0005692878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998746,0.000008199457,0.000005189608,0.000046955818,0.000036138736,0.000028907929],"domain_scores_gemma":[0.9998072,0.000014952269,0.000055585686,0.000029474159,0.000043441956,0.00004954702],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017837298,0.00034596573,0.00026152396,0.0006028107,0.00027999867,0.00054142426,0.00034670415,0.00034474983,0.0017660336],"category_scores_gemma":[0.00027675068,0.00021088909,0.00016360723,0.00063042186,0.00017725045,0.000231305,0.00044830597,0.00041028258,0.0006588513],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066628447,0.0002100808,0.5631749,0.00014324817,0.00015276868,0.00068843504,0.000377794,0.0034329405,0.39674807,0.00042752508,0.0025795458,0.03139837],"study_design_scores_gemma":[0.000028468587,0.00006326679,0.9885683,0.00001545238,0.000022230724,0.00016592369,0.00009167801,0.0022621374,0.0067400765,0.00007102904,0.001959993,0.000011419108],"about_ca_topic_score_codex":0.003555797,"about_ca_topic_score_gemma":0.008046216,"teacher_disagreement_score":0.003555797,"about_ca_system_score_codex":0.0004390177,"about_ca_system_score_gemma":0.00015892462,"threshold_uncertainty_score":0.0070702434},"labels":[],"label_agreement":null},{"id":"W4392376164","doi":"10.3847/1538-4357/ad13ea","title":"Explaining the GWSkyNet-Multi Machine Learning Classifier Predictions for Gravitational-wave Events","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Indo-US Science and Technology Forum; National Science Foundation","keywords":"Physics; Gravitational wave; Classifier (UML); Astronomy; Gravitation; Machine learning; Astrophysics; Artificial intelligence","score_opus":0.03626627206022515,"score_gpt":0.3441976928024399,"score_spread":0.30793142074221475,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392376164","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93416506,0.00026925185,0.058020648,0.0014494545,0.00011443248,0.00004270275,0.0021579247,0.0010515121,0.0027290497],"genre_scores_gemma":[0.9919704,0.000030900723,0.005613215,0.0000854051,0.000015754873,0.00002300621,0.0014113565,0.00003613184,0.0008138543],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979,0.000039857434,0.0000087387825,0.000068135734,0.000036663976,0.000056614434],"domain_scores_gemma":[0.99855167,0.00085708254,0.00013431597,0.00011283282,0.00024534477,0.00009880877],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010262111,0.00067608024,0.0003682565,0.0006189679,0.000336556,0.0007325606,0.0010377112,0.0010380988,0.0020940856],"category_scores_gemma":[0.003940444,0.00025948064,0.00037570516,0.00036079105,0.00044513206,0.0008348719,0.0005482662,0.0011436779,0.00051745493],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002820698,0.00015978352,0.07628005,0.00006223054,0.000060788858,0.00032081202,0.00009268389,0.87719655,0.0032563745,0.004816682,0.0063240286,0.031147962],"study_design_scores_gemma":[0.000003416269,0.0000084323165,0.0018373262,0.000004013573,0.0000019965573,0.000009076023,0.0000065532686,0.9962024,0.0005370685,0.0013040727,0.00008267175,0.0000030213978],"about_ca_topic_score_codex":0.011515002,"about_ca_topic_score_gemma":0.012567302,"teacher_disagreement_score":0.011515002,"about_ca_system_score_codex":0.001190377,"about_ca_system_score_gemma":0.00053990836,"threshold_uncertainty_score":0.022895932},"labels":[],"label_agreement":null},{"id":"W4392387174","doi":"10.3847/1538-4357/ad19db","title":"Powerful Radio-loud Quasars Are Triggered by Galaxy Mergers in the Cosmic Bright Ages","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Natural Sciences and Engineering Research Council of Canada; Space Telescope Science Institute; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Physics; Quasar; Astrophysics; Galaxy; COSMIC cancer database; Astronomy; Galaxy merger; Radio galaxy; X-shaped radio galaxy","score_opus":0.006636980570626812,"score_gpt":0.218400323788445,"score_spread":0.2117633432178182,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392387174","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939394,0.000082973864,0.000042863896,0.000018103337,0.0000026582343,0.0000015096886,0.00008354716,0.0000074468103,0.00036699855],"genre_scores_gemma":[0.9997979,0.000019401306,0.00001662133,0.000009772294,0.000007959136,7.1772547e-7,0.00007686783,9.868754e-7,0.000069891576],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989235,0.00001001663,0.000006577404,0.000032355798,0.000019473322,0.000039269387],"domain_scores_gemma":[0.99901605,0.00008444073,0.0005948283,0.000048236052,0.000043124404,0.00021328726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021957453,0.00021452353,0.00019752166,0.0013605601,0.00024842544,0.000661241,0.00018974618,0.00026792334,0.0015980288],"category_scores_gemma":[0.0004599927,0.00009913968,0.00014882315,0.00046703411,0.00038348293,0.0002456321,0.00035407263,0.00022673314,0.00018031542],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017684186,0.00004979314,0.9760188,0.000014006303,0.000036928766,0.00035771655,0.00021670756,0.00005916629,0.019879198,0.00010447092,0.0001541973,0.0029322307],"study_design_scores_gemma":[9.0456837e-7,0.000014891065,0.99956125,7.585319e-7,0.0000059866397,0.000081976425,0.000037011352,0.00003251952,0.00021003904,0.000010398494,0.000043429824,7.330435e-7],"about_ca_topic_score_codex":0.002380845,"about_ca_topic_score_gemma":0.0034716306,"teacher_disagreement_score":0.002380845,"about_ca_system_score_codex":0.0002062346,"about_ca_system_score_gemma":0.000064696076,"threshold_uncertainty_score":0.0053459406},"labels":[],"label_agreement":null},{"id":"W4392451591","doi":"10.3847/1538-4357/ad1bd0","title":"The Morphology of the Asteroidal Dust around White Dwarf Stars: Optical and Near-infrared Pulsations in G29-38","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"European Commission; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; White dwarf; Circumstellar dust; Astrophysics; Stars; Astronomy; Infrared; Cosmic dust; Infrared excess; Blue dwarf; Astrobiology","score_opus":0.00827454201808276,"score_gpt":0.22240111853775174,"score_spread":0.214126576519669,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392451591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997731,0.000016165443,0.000024869896,0.0000033813849,4.256915e-7,8.2382644e-7,0.000047768393,0.0000015999256,0.00013199066],"genre_scores_gemma":[0.9997894,0.000010070047,0.000041138937,0.0000027087738,0.0000013004154,8.956267e-7,0.000085193584,0.0000012296748,0.0000680102],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996245,0.0000031642612,0.000002907325,0.000015001616,0.000008408853,0.000008034995],"domain_scores_gemma":[0.9998715,0.000014990855,0.00005236381,0.000009482996,0.000016883885,0.000034707675],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008338131,0.00014239574,0.00015240387,0.0007117487,0.00021467784,0.00026555822,0.00020042583,0.00016921089,0.0005899835],"category_scores_gemma":[0.00017000805,0.000081680555,0.000106187494,0.00042762535,0.00021609812,0.00013865952,0.00031972074,0.00010842443,0.00019394039],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020077304,0.000030761308,0.916956,0.000011621708,0.000019354196,0.00059524487,0.00041899682,0.00015090649,0.07832804,0.000035156692,0.000052794167,0.0032003652],"study_design_scores_gemma":[0.0000012455415,0.000016128999,0.999153,5.760773e-7,0.0000021082524,0.00013297229,0.00007692184,0.0000697734,0.00048270094,0.0000113098895,0.000052378004,7.4340073e-7],"about_ca_topic_score_codex":0.003157662,"about_ca_topic_score_gemma":0.004078845,"teacher_disagreement_score":0.003157662,"about_ca_system_score_codex":0.0002012059,"about_ca_system_score_gemma":0.00005145816,"threshold_uncertainty_score":0.0062785745},"labels":[],"label_agreement":null},{"id":"W4392451704","doi":"10.3847/1538-4357/ad198c","title":"Long-term Evolution in Ionization of Ejecta Illuminated by Eta Carinae","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Ejecta; Term (time); Ionization; Astrophysics; Astronomy; Supernova; Ion","score_opus":0.006408329905041199,"score_gpt":0.22843077539213646,"score_spread":0.22202244548709527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392451704","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992231,0.00016547431,0.000020630438,0.000015744654,0.0000022339466,0.0000011394692,0.00019164881,0.0000029126238,0.00037709414],"genre_scores_gemma":[0.9989806,0.00007745966,0.000023612196,0.000008254567,0.0000043850755,0.0000016636045,0.00046956717,0.0000027335918,0.000431661],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993134,0.0000062419927,0.0000035611824,0.000023177488,0.000013529808,0.000022049651],"domain_scores_gemma":[0.9996586,0.000026799013,0.0001210914,0.000013202155,0.00007020702,0.000110098845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010869223,0.00014977541,0.00018092405,0.0005659566,0.00034770512,0.000638963,0.00016593574,0.00027479217,0.0019459438],"category_scores_gemma":[0.00044230805,0.00008728666,0.00012110054,0.00038639075,0.00013498285,0.00026872227,0.00038773456,0.00028721776,0.00044602194],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020804843,0.0000636861,0.9852485,0.00001711096,0.00005714412,0.0002734106,0.00031287994,0.00015440202,0.009503842,0.000038092337,0.00021737038,0.0039053902],"study_design_scores_gemma":[3.545763e-7,0.000007640424,0.999537,0.0000015160557,0.0000030743038,0.000046425892,0.00008380284,0.000046082532,0.00013148277,0.0000049095993,0.0001368205,0.000001072104],"about_ca_topic_score_codex":0.0057265614,"about_ca_topic_score_gemma":0.007113385,"teacher_disagreement_score":0.0057265614,"about_ca_system_score_codex":0.0003895099,"about_ca_system_score_gemma":0.0000838687,"threshold_uncertainty_score":0.011386514},"labels":[],"label_agreement":null},{"id":"W4392451916","doi":"10.3847/1538-4357/ad1ffd","title":"The DESI One-percent Survey: Evidence for Assembly Bias from Low-redshift Counts-in-cylinders Measurements","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Division of Astronomical Sciences; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministerio de Ciencia e Innovación; National Science Foundation; Consejo Nacional de Ciencia y Tecnología; U.S. Department of Energy; Gordon and Betty Moore Foundation; Office of Science; National Aeronautics and Space Administration","keywords":"Physics; Halo; Astrophysics; Redshift; Galaxy; Halo effect; Luminosity","score_opus":0.1011836257867257,"score_gpt":0.30040042131634365,"score_spread":0.19921679552961796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392451916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97691387,0.00035660004,0.014135849,0.00027759385,0.00002478933,0.000014429444,0.0039908323,0.0012996858,0.0029863282],"genre_scores_gemma":[0.99437886,0.00003693034,0.0018416905,0.000096911856,0.000010756047,0.000008577979,0.003188441,0.00017955732,0.00025829783],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987074,0.0005148286,0.00005059802,0.00033344986,0.00023123802,0.0001624874],"domain_scores_gemma":[0.9939448,0.0026730644,0.001158355,0.0012787203,0.0005420896,0.00040292667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0035506664,0.0004721745,0.00057070423,0.0008528181,0.00040250536,0.0010531172,0.0010874547,0.0005370621,0.0026043432],"category_scores_gemma":[0.013112167,0.00033254785,0.0006114178,0.0009630472,0.0007966851,0.0008075509,0.0010205937,0.0006320622,0.00086206995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027853748,0.00003121339,0.9420678,0.000085416075,0.00019406313,0.00010403342,0.0002536734,0.03347302,0.0021138797,0.0035893929,0.0053477003,0.012461263],"study_design_scores_gemma":[0.0000701712,0.0001319706,0.61238396,0.00012558064,0.00013440523,0.00038489018,0.00044576544,0.35745808,0.00567127,0.009798012,0.013320964,0.00007503971],"about_ca_topic_score_codex":0.017019507,"about_ca_topic_score_gemma":0.017195484,"teacher_disagreement_score":0.017019507,"about_ca_system_score_codex":0.00071629824,"about_ca_system_score_gemma":0.00046394803,"threshold_uncertainty_score":0.033840895},"labels":[],"label_agreement":null},{"id":"W4392451917","doi":"10.3847/1538-4357/ad18b9","title":"The ALMaQUEST Survey. XII. Dense Molecular Gas as Traced by HCN and HCO<sup>+</sup> in Green Valley Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Academia Sinica","keywords":"Physics; Galaxy; Astrophysics; Astronomy","score_opus":0.006048156675028782,"score_gpt":0.21669687595298034,"score_spread":0.21064871927795156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392451917","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968928,0.00014038275,0.000042021267,0.000033204364,0.0000022662625,0.0000026586868,0.0020165402,0.000020086485,0.00085001666],"genre_scores_gemma":[0.99493754,0.00007302285,0.00020984549,0.000047073816,0.000009935268,0.000004510769,0.0041951095,0.0000111846575,0.00051179755],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986887,0.000017009823,0.0000040626815,0.000047741272,0.000028587712,0.000033652126],"domain_scores_gemma":[0.99938977,0.00005572093,0.00025245702,0.000058416867,0.00008725513,0.00015639904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023406351,0.0001309962,0.00015450857,0.0010541731,0.00022964965,0.00047527862,0.00028117088,0.00019910527,0.0010847765],"category_scores_gemma":[0.0003147571,0.000077240555,0.0001927355,0.00081328175,0.00020972987,0.00020375154,0.00033350158,0.00013365557,0.0003453946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000089357796,0.000018614839,0.98972356,0.000015433567,0.00004735679,0.00007726336,0.00020249709,0.000082451465,0.003460452,0.00007397572,0.0009800771,0.0052289125],"study_design_scores_gemma":[0.000004856332,0.0000125615525,0.99862623,0.0000015445397,0.0000060098855,0.00003251015,0.000097230535,0.00012118505,0.00016382722,0.000017789747,0.00091473135,0.0000014936951],"about_ca_topic_score_codex":0.020665195,"about_ca_topic_score_gemma":0.061061583,"teacher_disagreement_score":0.020665195,"about_ca_system_score_codex":0.00035156024,"about_ca_system_score_gemma":0.00018286583,"threshold_uncertainty_score":0.041089833},"labels":[],"label_agreement":null},{"id":"W4392513748","doi":"10.3847/1538-4357/ad192c","title":"A First Look with JWST Aperture Masking Interferometry: Resolving Circumstellar Dust around the Wolf–Rayet Binary WR 137 beyond the Rayleigh Limit","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Natural Sciences and Engineering Research Council of Canada; Goddard Space Flight Center; Space Telescope Science Institute; Research Corporation for Science Advancement; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Observable; Circumstellar dust; Spectrograph; Astronomy; Interferometry; Orbital plane; Stars; Spectral line","score_opus":0.009940643957036829,"score_gpt":0.21831922894273784,"score_spread":0.208378584985701,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392513748","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958813,0.000055424058,0.0023533825,0.000038459868,0.0000034199622,0.0000074213654,0.00021116972,0.00017271681,0.0012767151],"genre_scores_gemma":[0.99336594,0.00001886628,0.0059966817,0.000017101265,0.000009369496,0.00000418341,0.0003765714,0.000040974854,0.00017023153],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999293,0.000009385194,0.0000040666528,0.000019754529,0.000022980983,0.000014537891],"domain_scores_gemma":[0.99979943,0.000046617966,0.00003409144,0.00004721429,0.00003346092,0.000039207065],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036291013,0.00015180618,0.00018869057,0.00044674147,0.00023139964,0.00043642963,0.00034111517,0.00018345192,0.0010481387],"category_scores_gemma":[0.00048330493,0.00013317431,0.00025203315,0.00029581523,0.000119258184,0.00026476593,0.00032979378,0.00024232338,0.00019588358],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000992292,0.0001558523,0.5091694,0.00010688622,0.00019800996,0.00096264144,0.00065103656,0.0062279245,0.4189781,0.0011203457,0.0014597159,0.059977837],"study_design_scores_gemma":[0.000042740463,0.0002372708,0.937095,0.000018959636,0.00007058791,0.0003829731,0.00018621662,0.02765562,0.030831344,0.00037213022,0.00308494,0.000022145354],"about_ca_topic_score_codex":0.0016289869,"about_ca_topic_score_gemma":0.0036305266,"teacher_disagreement_score":0.0016289869,"about_ca_system_score_codex":0.00019356722,"about_ca_system_score_gemma":0.00011281223,"threshold_uncertainty_score":0.003506422},"labels":[],"label_agreement":null},{"id":"W4392517068","doi":"10.3847/1538-4357/ad2171","title":"GBT/Argus Observations of Molecular Gas in the Inner Regions of IC 342","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Science Foundation","keywords":"Argus; Physics; Astronomy; Astrobiology; Astrophysics","score_opus":0.020203025649102795,"score_gpt":0.25422616440822904,"score_spread":0.23402313875912625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392517068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955609,0.000058555135,0.00029368565,0.00005982677,0.000004803978,0.000006276692,0.0010086423,0.00034018265,0.0026672306],"genre_scores_gemma":[0.99724054,0.00003453747,0.00063918554,0.000038972987,0.000016598986,0.000007727974,0.001426415,0.000028990671,0.0005670111],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99990296,0.0000069446,0.0000018640334,0.00002407386,0.000034794004,0.000029274464],"domain_scores_gemma":[0.999887,0.000008006592,0.000031391264,0.000016628757,0.000018394056,0.00003869478],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000117021176,0.00022961374,0.0002195419,0.0010653113,0.00037822104,0.00030856128,0.00030311584,0.00024032393,0.0019291322],"category_scores_gemma":[0.00022950364,0.00021027248,0.00016401272,0.0006386318,0.00022539655,0.00016934954,0.00048540032,0.00027249215,0.00038462487],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013218138,0.00019786075,0.45629582,0.0001350543,0.00019273027,0.0010336943,0.00062729075,0.005733249,0.48006588,0.0010684986,0.013642949,0.039685216],"study_design_scores_gemma":[0.000049395087,0.000043508448,0.9903116,0.0000060234215,0.000026948055,0.00009719112,0.000054016084,0.0017874233,0.0048384853,0.00009754788,0.0026757184,0.000012026885],"about_ca_topic_score_codex":0.01567811,"about_ca_topic_score_gemma":0.022014488,"teacher_disagreement_score":0.01567811,"about_ca_system_score_codex":0.0005625871,"about_ca_system_score_gemma":0.0001603003,"threshold_uncertainty_score":0.031173706},"labels":[],"label_agreement":null},{"id":"W4392517568","doi":"10.3847/1538-4357/ad1be4","title":"AGN STORM 2. V. Anomalous Behavior of the C <scp>iv</scp> Light Curve of Mrk 817*","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; University of California, Irvine; Israel Science Foundation; Chinese Academy of Sciences; National Natural Science Foundation of China; Gordon and Betty Moore Foundation; Nuclear Safety and Security Commission; Consejo Nacional de Ciencia y Tecnología; Space Telescope Science Institute; Alexander von Humboldt-Stiftung; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; National Aeronautics and Space Administration; Wayne State University; National Science Foundation","keywords":"Physics; Light curve; Astrophysics; Galaxy; Emission spectrum; Spectral line; Outflow; Astronomy; Line (geometry); Hubble space telescope; Spectral energy distribution; Active galactic nucleus","score_opus":0.0066760673483209345,"score_gpt":0.21349191358878714,"score_spread":0.2068158462404662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392517568","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99836487,0.000020028303,0.00011424006,0.00002067777,0.0000026239588,0.000003073441,0.00029460888,0.00003708195,0.0011429427],"genre_scores_gemma":[0.99915695,0.0000051277393,0.0000785247,0.0000086865,0.0000035611474,0.0000019813078,0.0005006971,0.0000042681554,0.00024020285],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992836,0.0000039099295,0.0000029920573,0.000021907326,0.000017203804,0.000025692403],"domain_scores_gemma":[0.9996138,0.000045806733,0.00012099364,0.00003459501,0.00006230048,0.00012258986],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012960116,0.00011312667,0.00015825639,0.0004403749,0.00025068125,0.00042250002,0.00014795763,0.0002647003,0.0011886331],"category_scores_gemma":[0.0003505736,0.00006192907,0.00009487834,0.00021624715,0.00012566925,0.00012645926,0.00023472389,0.00025561522,0.0004209743],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004398579,0.00015309498,0.8901045,0.00003900009,0.0000627388,0.0010340734,0.00033781666,0.0012902339,0.088480055,0.000509045,0.0019218435,0.015627705],"study_design_scores_gemma":[0.0000022572888,0.000040655952,0.9971238,0.0000014139448,0.0000035525522,0.0001126067,0.00004293715,0.00078989397,0.0014080451,0.000026227437,0.00044556207,0.000003141605],"about_ca_topic_score_codex":0.0039680745,"about_ca_topic_score_gemma":0.0039220466,"teacher_disagreement_score":0.0039680745,"about_ca_system_score_codex":0.00033017318,"about_ca_system_score_gemma":0.00010061896,"threshold_uncertainty_score":0.007889926},"labels":[],"label_agreement":null},{"id":"W4392554302","doi":"10.3847/1538-4357/ad1f61","title":"The NANOGrav 12.5 yr Data Set: A Computationally Efficient Eccentric Binary Search Pipeline and Constraints on an Eccentric Supermassive Binary Candidate in 3C 66B","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Particle physics theoretical and experimental studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Office of Naval Research; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; Israel Academy of Sciences and Humanities; College of Science, Oregon State University; Alfred P. Sloan Foundation; Brinson Foundation; Goddard Space Flight Center; Jet Propulsion Laboratory; Council for Higher Education; Department of Atomic Energy, Government of India; Space Telescope Science Institute; Oregon State University; Canadian Institute for Advanced Research; Associated Universities; Texas Tech University; West Virginia University; Vanderbilt University; University of Toronto; Flatiron Health; National Aeronautics and Space Administration; Research Corporation for Science Advancement; Deutsche Forschungsgemeinschaft; University of Central Florida; National Science Foundation","keywords":"Physics; Eccentric; Binary number; Astrophysics; Set (abstract data type); Data set; Supermassive black hole; Pipeline (software); Astronomy; Galaxy; Artificial intelligence","score_opus":0.020901156604246726,"score_gpt":0.30013548489146397,"score_spread":0.2792343282872172,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392554302","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97790396,0.0001324169,0.01063419,0.00034003909,0.000027012366,0.00008892527,0.0054132086,0.002646209,0.0028139977],"genre_scores_gemma":[0.9196436,0.00004748967,0.052156605,0.00017004936,0.000019652454,0.00009886357,0.026498483,0.0003090253,0.001056287],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9997247,0.000052714044,0.00001569535,0.00007732938,0.00008912831,0.000040408933],"domain_scores_gemma":[0.99926347,0.00029482512,0.000084559084,0.00010918449,0.00012681396,0.000121121135],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009116251,0.0006652086,0.0006193107,0.0011371878,0.00076703134,0.0008353111,0.0013892401,0.0008407616,0.002241782],"category_scores_gemma":[0.002240913,0.0004526631,0.0007578813,0.0009114553,0.0003993486,0.00072705647,0.0009966671,0.00059475336,0.00065278885],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0036027827,0.001364716,0.16157821,0.0004309537,0.00076065084,0.0018102598,0.00052542274,0.6425364,0.05862145,0.0050990186,0.021689842,0.10198031],"study_design_scores_gemma":[0.00036580794,0.00019004886,0.018615557,0.000011215285,0.000039987175,0.00012562698,0.00012765412,0.97056377,0.0059416364,0.0013230358,0.0026555161,0.00004014992],"about_ca_topic_score_codex":0.018761065,"about_ca_topic_score_gemma":0.03817484,"teacher_disagreement_score":0.018761065,"about_ca_system_score_codex":0.0007179538,"about_ca_system_score_gemma":0.0012694364,"threshold_uncertainty_score":0.037303746},"labels":[],"label_agreement":null},{"id":"W4392560250","doi":"10.3847/1538-4357/ad235a","title":"X-Ray Polarimetry of the Dipping Accreting Neutron Star 4U 1624–49","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; RIKEN; Istituto Nazionale di Fisica Nucleare; Japan Aerospace Exploration Agency; Ministero degli Affari Esteri e della Cooperazione Internazionale; Agenzia Spaziale Italiana; Deutscher Akademischer Austauschdienst; Istituto Nazionale di Astrofisica; Marshall Space Flight Center; National Aeronautics and Space Administration","keywords":"Physics; Neutron star; Astrophysics; Polarimetry; X-ray binary; Astronomy; X-ray; X-ray burster; Star (game theory); Binary star; Nuclear physics; Stars; Stellar evolution; Scattering; Stellar mass loss; Optics","score_opus":0.011107507521747608,"score_gpt":0.236539163521693,"score_spread":0.22543165599994539,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392560250","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99603975,0.00016757184,0.0007249726,0.000022614886,0.0000072340545,0.000010330217,0.00030820823,0.000042970798,0.0026763722],"genre_scores_gemma":[0.99738055,0.00006592118,0.0014015827,0.000022755736,0.000011540585,0.000006834251,0.00066534843,0.000017200948,0.00042826487],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99987125,0.000019738429,0.0000064968567,0.00003780258,0.000042981123,0.000021552534],"domain_scores_gemma":[0.99969256,0.00004216686,0.00011253422,0.00004166106,0.00005187751,0.00005930951],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033666092,0.00029853993,0.00038109988,0.0009336455,0.00043979345,0.0005922994,0.0002502867,0.0003203716,0.0012551765],"category_scores_gemma":[0.00052272953,0.00026115595,0.00016136198,0.0005699079,0.00033446157,0.00024803492,0.000654313,0.00036293367,0.00038708845],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00097212684,0.00010521562,0.39492023,0.00011484133,0.00015415336,0.0016926179,0.0002974505,0.0025784015,0.57814354,0.0005329326,0.00055670633,0.019931763],"study_design_scores_gemma":[0.000028514767,0.00021848889,0.9751052,0.000014232245,0.000035387573,0.0007696815,0.00012116829,0.0025395663,0.01905996,0.00017189146,0.0019219269,0.000013997837],"about_ca_topic_score_codex":0.0011963506,"about_ca_topic_score_gemma":0.0015413256,"teacher_disagreement_score":0.0012551765,"about_ca_system_score_codex":0.0002818029,"about_ca_system_score_gemma":0.00012766443,"threshold_uncertainty_score":0.004199028},"labels":[],"label_agreement":null},{"id":"W4392587961","doi":"10.3847/1538-4357/ad29f7","title":"Erratum: “Spacetime Metrics and Ringdown Waveforms for Galactic Black Holes Surrounded by a Dark Matter Spike” (2022, ApJ, 940, 33)","year":2024,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Winnipeg","funders":"Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Spike (software development); Dark matter; Spacetime; Astronomy; Quantum mechanics","score_opus":0.011953208924968305,"score_gpt":0.24063181276144804,"score_spread":0.22867860383647973,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392587961","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.007501484,0.0016803335,0.0060468907,0.07830124,0.77876556,0.000082260995,0.019264748,0.0027237856,0.105633646],"genre_scores_gemma":[0.09415276,0.0025138129,0.015823528,0.043038618,0.08001498,0.00014889744,0.02686245,0.0040184273,0.7334265],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9996586,0.00004426516,0.000046040168,0.00006298258,0.00015752141,0.000030598894],"domain_scores_gemma":[0.99734193,0.0006074956,0.00020030586,0.00022746058,0.0014035797,0.00021926468],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000613139,0.0011946236,0.00048561455,0.001746407,0.002008295,0.002317964,0.0011534836,0.002148384,0.08301596],"category_scores_gemma":[0.009757228,0.00038331316,0.00063001853,0.0012160735,0.00078938785,0.0019939088,0.0008656774,0.0022741507,0.03029206],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000073686955,0.000005431307,0.00024447995,0.0000292215,0.0000047453955,0.0002990644,0.00002420993,0.00011993355,0.00018349737,0.0036497507,0.99095684,0.004409194],"study_design_scores_gemma":[0.000090696485,0.000067881454,0.008216421,0.0001689288,0.000035444504,0.0012387398,0.0002953327,0.0019703112,0.0011809159,0.017238487,0.9694025,0.00009432723],"about_ca_topic_score_codex":0.016974343,"about_ca_topic_score_gemma":0.01787052,"teacher_disagreement_score":0.08301596,"about_ca_system_score_codex":0.0012471599,"about_ca_system_score_gemma":0.0010197379,"threshold_uncertainty_score":0.27771604},"labels":[],"label_agreement":null},{"id":"W4392588094","doi":"10.3847/1538-4357/ad151d","title":"The Disk Orientations of Perseus Protostellar Multiples at ∼8 au Resolution","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Angular resolution (graph drawing); Interstellar medium; Astronomical spectroscopy; Stars; Galaxy","score_opus":0.011914676006938005,"score_gpt":0.25911120032940077,"score_spread":0.24719652432246275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392588094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989875,0.000051356656,0.00035190687,0.00000834239,0.000001253662,0.0000015149245,0.00031188581,0.000029275905,0.0002568438],"genre_scores_gemma":[0.99910223,0.000016224907,0.0003316844,0.000004331354,0.000003727727,0.0000017631876,0.0004584612,0.0000054663296,0.00007621592],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988556,0.000010258656,0.0000059320646,0.000056959252,0.000026766882,0.000014476326],"domain_scores_gemma":[0.99926955,0.00015741326,0.00023653053,0.00011048315,0.00012976796,0.000096235075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019299498,0.00014539558,0.0001765713,0.00082836405,0.00020677055,0.0003203682,0.0001789498,0.00010233077,0.0010655929],"category_scores_gemma":[0.0009381562,0.00009697604,0.00017963722,0.0005850939,0.00019207013,0.00020717808,0.00027041393,0.00014686,0.00028594045],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012972364,0.000019462583,0.9646158,0.0000150456435,0.00006621744,0.0001040445,0.0000912009,0.0024592655,0.019112082,0.00013892465,0.00032250438,0.012925588],"study_design_scores_gemma":[0.000002854533,0.000015380552,0.9945792,0.0000014376798,0.000008460446,0.0000904562,0.000042962245,0.003390667,0.001519958,0.00007428741,0.0002714847,0.0000028649324],"about_ca_topic_score_codex":0.0025659266,"about_ca_topic_score_gemma":0.0029704578,"teacher_disagreement_score":0.0025659266,"about_ca_system_score_codex":0.00019417796,"about_ca_system_score_gemma":0.00006202175,"threshold_uncertainty_score":0.005101979},"labels":[],"label_agreement":null},{"id":"W4392646466","doi":"10.3847/1538-4357/ad1ff4","title":"Orbital Stability and Secular Dynamics of the Proxima Centauri Planetary System","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration","keywords":"Physics; Planet; Astrophysics; Celestial mechanics; Astronomy; Planetary system; Orbital elements; Stability (learning theory); Orbital mechanics; Exoplanet; Gravitation; Satellite","score_opus":0.006313213122326078,"score_gpt":0.19436296451067414,"score_spread":0.18804975138834806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392646466","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989767,0.0000764747,0.00012968229,0.000019712254,0.0000012412571,7.623062e-7,0.000074686,0.0000066270527,0.0007141199],"genre_scores_gemma":[0.9998196,0.000013584225,0.00003075887,0.0000011479427,9.0697404e-7,4.0580457e-7,0.00005818978,0.0000017160648,0.00007378994],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999293,0.000014655965,0.0000056047065,0.000021695258,0.000014597128,0.000014175534],"domain_scores_gemma":[0.9988599,0.00023798202,0.000427604,0.000090789144,0.0002060219,0.00017771142],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033920672,0.00013006951,0.00016563619,0.0013959443,0.00031002384,0.00082255487,0.0001458598,0.0002196047,0.0014810059],"category_scores_gemma":[0.0023664143,0.00009379776,0.00010815481,0.00059596996,0.0003843122,0.00041422155,0.0006030204,0.00017849226,0.00031037783],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031236562,0.000026428452,0.9590407,0.000036816426,0.000111267196,0.00017586089,0.0006862571,0.009114056,0.017824208,0.0018994355,0.00027238156,0.010500213],"study_design_scores_gemma":[0.0000052062874,0.00006657232,0.97692186,0.000008341113,0.000021581951,0.00016172885,0.00030354742,0.0193104,0.0017828705,0.0008967764,0.00050863053,0.0000126130835],"about_ca_topic_score_codex":0.0027359948,"about_ca_topic_score_gemma":0.0017466473,"teacher_disagreement_score":0.0027359948,"about_ca_system_score_codex":0.0003084745,"about_ca_system_score_gemma":0.0001167627,"threshold_uncertainty_score":0.005440116},"labels":[],"label_agreement":null},{"id":"W4392703586","doi":"10.3847/1538-4357/ad2209","title":"Probing the Global 21 cm Background by Velocity-induced Dipole and Quadrupole Anisotropies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"National Research Foundation of Korea; Johns Hopkins University","keywords":"Physics; Quadrupole; Dipole; Anisotropy; Astrophysics; Background radiation; Astronomy; Atomic physics; Nuclear physics; Optics; Quantum mechanics; Radiation","score_opus":0.013176553862914737,"score_gpt":0.24761090282798878,"score_spread":0.23443434896507404,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392703586","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94014347,0.0013116343,0.03941233,0.00044645986,0.00012129286,0.000028003846,0.0009822225,0.00056547613,0.01698921],"genre_scores_gemma":[0.9953766,0.0002200336,0.0031834263,0.00009009902,0.00003993562,0.000006657346,0.0003525878,0.000055387463,0.00067518547],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997917,0.000028651772,0.0000041164913,0.00008213323,0.000045737394,0.00004764635],"domain_scores_gemma":[0.9993376,0.0001208585,0.00024311346,0.00010110228,0.00009868163,0.00009865444],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047913846,0.00041198215,0.00017315373,0.0005679614,0.00025496073,0.0005586716,0.0002847584,0.00033542752,0.0030893805],"category_scores_gemma":[0.00113787,0.00017750784,0.0001780632,0.0005001542,0.00037454756,0.00055042485,0.0007179525,0.00043395962,0.00045744475],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005558559,0.000082014994,0.18355353,0.0001762989,0.000198497,0.0002038508,0.00021478535,0.0064588436,0.7395348,0.010839559,0.0016333769,0.056548536],"study_design_scores_gemma":[0.000064691,0.00053584017,0.8484251,0.00006360448,0.0001693396,0.0005143524,0.00027266907,0.021072986,0.10585841,0.008996883,0.013919551,0.000106682244],"about_ca_topic_score_codex":0.00094339804,"about_ca_topic_score_gemma":0.0020272252,"teacher_disagreement_score":0.0030893805,"about_ca_system_score_codex":0.0004230205,"about_ca_system_score_gemma":0.00016135353,"threshold_uncertainty_score":0.010334969},"labels":[],"label_agreement":null},{"id":"W4392715743","doi":"10.3847/1538-4357/ad26fb","title":"Study of Plasma Heating Processes in a Coronal Mass Ejection–driven Shock Sheath Region Observed with the Metis Coronagraph","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Bundesministerium für Wirtschaft und Energie; Istituto Nazionale di Astrofisica; National Aeronautics and Space Administration","keywords":"Physics; Coronal mass ejection; Coronagraph; Astrophysics; Heliosphere; Shock (circulatory); Shock wave; Astronomy; Solar flare; Solar wind; Plasma; Exoplanet; Mechanics; Stars","score_opus":0.019388116126111056,"score_gpt":0.23868481124137989,"score_spread":0.21929669511526884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392715743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988165,0.00007610922,0.00037351827,0.000010786238,0.000001979615,0.000004923905,0.000115416304,0.000018988803,0.0005817574],"genre_scores_gemma":[0.99930084,0.000026402226,0.00035542212,0.0000061644178,0.0000053034987,0.0000027762903,0.00013807825,0.0000044941835,0.0001604945],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999714,0.0000024033354,7.9549136e-7,0.000008330792,0.000008593183,0.0000084547555],"domain_scores_gemma":[0.9999248,0.000018319715,0.000018109118,0.0000068115583,0.000012662485,0.000019310211],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007467904,0.00011212211,0.00012238669,0.00043205038,0.00019207726,0.00019183988,0.00013961304,0.00021133272,0.0004958653],"category_scores_gemma":[0.00012720498,0.000087385095,0.00013711961,0.00026532868,0.00009339799,0.000112337424,0.00012365064,0.00016826452,0.000080594415],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049483136,0.00007566516,0.2175014,0.000046078396,0.00007616078,0.001190476,0.0005920639,0.0011949427,0.7650206,0.00019563745,0.00036432053,0.013247703],"study_design_scores_gemma":[0.000009826951,0.00013367731,0.97217935,0.0000037633226,0.00002068172,0.0003381441,0.00014956221,0.004747003,0.021696264,0.000039687984,0.000674498,0.0000074866957],"about_ca_topic_score_codex":0.0018371423,"about_ca_topic_score_gemma":0.0026167687,"teacher_disagreement_score":0.0018371423,"about_ca_system_score_codex":0.00017248535,"about_ca_system_score_gemma":0.00005915183,"threshold_uncertainty_score":0.0036528707},"labels":[],"label_agreement":null},{"id":"W4392736400","doi":"10.3847/1538-4357/ad4d8e","title":"Performance of SK-Gd’s Upgraded Real-time Supernova Monitoring System","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Institute for Basic Science; Ministry of Education, Culture, Sports, Science and Technology; Japan Society for the Promotion of Science; Horizon 2020 Framework Programme; Science and Technology Facilities Council; National Research Foundation; U.S. Department of Energy; European Commission; Western Canada Research Grid; National Natural Science Foundation of China; National Science Foundation; Compute Canada; National Research Foundation of Korea","keywords":"Supernova; Physics; Neutrino; Astrophysics; Galaxy; Astronomy; Nuclear physics","score_opus":0.008273456926839102,"score_gpt":0.21854376324050145,"score_spread":0.21027030631366236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392736400","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9599809,0.00016202449,0.013729068,0.00008233804,0.00014292462,0.000109040666,0.0011616161,0.020453813,0.0041782265],"genre_scores_gemma":[0.99262977,0.000020842373,0.004514378,0.000043641205,0.000010088165,0.000021059539,0.0012470061,0.00014765502,0.0013655116],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99899596,0.00012563802,0.00007414608,0.00035251732,0.00031561937,0.00013605387],"domain_scores_gemma":[0.99844956,0.00021573562,0.0001549121,0.00034344406,0.0006120676,0.00022426667],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009965147,0.0007246141,0.00048451085,0.000867809,0.00020128551,0.00050823524,0.0009644539,0.00045206974,0.002871979],"category_scores_gemma":[0.0022806688,0.00022127984,0.00030116542,0.00037992455,0.00018712945,0.00047750393,0.0006869992,0.00038608973,0.0017555611],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.014939085,0.0014520129,0.23511252,0.0006545734,0.00064308435,0.0015673846,0.0009144779,0.09699649,0.2763181,0.0011992144,0.031057628,0.3391455],"study_design_scores_gemma":[0.00045686707,0.0023698932,0.15613246,0.000052386484,0.00022330675,0.0005886133,0.00017655148,0.6803942,0.14235114,0.00023907596,0.016838586,0.0001770732],"about_ca_topic_score_codex":0.004835838,"about_ca_topic_score_gemma":0.0021863698,"teacher_disagreement_score":0.004835838,"about_ca_system_score_codex":0.0005678023,"about_ca_system_score_gemma":0.00039221335,"threshold_uncertainty_score":0.009615421},"labels":[],"label_agreement":null},{"id":"W4392737529","doi":"10.3847/1538-4357/ad344d","title":"Tidal Synchronization Trapping in Stars and Planets with Convective Envelopes","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Planet; Rotation (mathematics); Stars; Inertial wave; Astrophysics; Exoplanet; Amplitude; Geometry","score_opus":0.006361203137696738,"score_gpt":0.20393000363566,"score_spread":0.19756880049796327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392737529","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9945754,0.00008813515,0.0042123524,0.00004296298,0.00000589646,0.0000039479055,0.000025618772,0.000049124166,0.000996513],"genre_scores_gemma":[0.99956995,0.000012375918,0.0002798093,0.000003747877,0.0000021727883,0.0000011792588,0.000013217324,0.0000036754006,0.00011390085],"study_design_codex":"bench_or_experimental","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999417,0.0000067815918,0.00000412009,0.000017691505,0.000016252608,0.0000134658185],"domain_scores_gemma":[0.99934,0.00012817785,0.00029731952,0.0000996518,0.00004505907,0.00008980366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020102045,0.00011717069,0.00021828034,0.00042047357,0.0004959695,0.00053067465,0.00023277849,0.00022846943,0.0009630242],"category_scores_gemma":[0.0011798077,0.00014407758,0.000122061174,0.00023266797,0.0006292633,0.00058230414,0.00063003233,0.00020191485,0.00011586199],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011499574,0.00027080128,0.3187309,0.00020480686,0.00020810074,0.0017535852,0.0013946537,0.13159038,0.41959912,0.07417175,0.0018358671,0.049090028],"study_design_scores_gemma":[0.00012420777,0.00048674224,0.1564616,0.00002951305,0.00006902821,0.0011716334,0.00047167495,0.67771906,0.10046388,0.05880307,0.0041474164,0.000052192114],"about_ca_topic_score_codex":0.0008650714,"about_ca_topic_score_gemma":0.00038833404,"teacher_disagreement_score":0.0009630242,"about_ca_system_score_codex":0.00033973972,"about_ca_system_score_gemma":0.0001501051,"threshold_uncertainty_score":0.0032216907},"labels":[],"label_agreement":null},{"id":"W4392768625","doi":"10.3847/1538-4357/ad21e3","title":"Multiple Jets in the Bursting Protostar HOPS 373SW","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Korea Astronomy and Space Science Institute","keywords":"Physics; Astrophysics; Outflow; Protostar; Submillimeter Array; Millimeter; Sky; Astronomy; Jet (fluid); Brightness; Accretion (finance); Bow shock (aerodynamics); Star formation; Shock wave; Stars","score_opus":0.015352073215262826,"score_gpt":0.25873171411485146,"score_spread":0.24337964089958863,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392768625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99964535,0.000022886457,0.000040683004,0.000006901953,0.0000016161889,0.0000010384864,0.000051818784,0.000008055169,0.0002216207],"genre_scores_gemma":[0.9995802,0.000013192738,0.00009293114,0.000007647395,0.000001974056,0.000001124172,0.0001112377,0.0000025914744,0.00018916343],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999966,0.0000014505387,0.0000020230575,0.000008980317,0.000009816319,0.000011693199],"domain_scores_gemma":[0.9998534,0.000013260658,0.000041641102,0.000011294128,0.000014034313,0.000066346875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00004764619,0.00016038929,0.00018341554,0.00048042953,0.0003547416,0.00038790892,0.00013488713,0.0002826718,0.0010401282],"category_scores_gemma":[0.00014213283,0.00012499688,0.00014685119,0.00033868567,0.0002677367,0.00011538513,0.0004505322,0.00016201274,0.00018409114],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091292075,0.00008836891,0.62894243,0.000053606997,0.00007392511,0.019006036,0.000981233,0.0012616114,0.33335412,0.0006018607,0.00061583205,0.014108126],"study_design_scores_gemma":[0.000027535647,0.00030439923,0.9752354,0.0000146705315,0.000035522346,0.0048479266,0.0009767691,0.0014811505,0.014653397,0.00039173182,0.0020126384,0.00001888421],"about_ca_topic_score_codex":0.0040190467,"about_ca_topic_score_gemma":0.0071857893,"teacher_disagreement_score":0.0040190467,"about_ca_system_score_codex":0.00031488494,"about_ca_system_score_gemma":0.0001238796,"threshold_uncertainty_score":0.007991314},"labels":[],"label_agreement":null},{"id":"W4392769258","doi":"10.3847/1538-4357/ad18d6","title":"Search for Continuous and Transient Neutrino Emission Associated with IceCube’s Highest-energy Tracks: An 11 yr Analysis","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Alliance de recherche numérique du Canada; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Fonds Wetenschappelijk Onderzoek; Nvidia; Marquette University","keywords":"Physics; Neutrino; Blazar; Astrophysics; Flux (metallurgy); Event (particle physics); Transient (computer programming); Neutrino astronomy; Neutrino detector; Energy (signal processing); Astronomy; Nuclear physics; Neutrino oscillation; Gamma ray","score_opus":0.009476804155200087,"score_gpt":0.23674057710366195,"score_spread":0.22726377294846187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392769258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951363,0.00012701332,0.0007886553,0.00002941886,0.0000073316965,0.0000107167025,0.0025467724,0.0000371668,0.001316682],"genre_scores_gemma":[0.98665243,0.0000888872,0.001132704,0.000037076177,0.000024275483,0.000018320849,0.011228752,0.00003390718,0.0007837377],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99962187,0.00007756677,0.000019001813,0.000113273054,0.00008561159,0.00008279018],"domain_scores_gemma":[0.99835485,0.0006878931,0.00046908224,0.00016358368,0.00014158471,0.00018295638],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00093267905,0.00033930907,0.00040565748,0.0011116894,0.00030935952,0.00089429267,0.00028407451,0.00024198099,0.0025567818],"category_scores_gemma":[0.0013011625,0.00012910248,0.0006376484,0.0010107057,0.00022630315,0.00032462025,0.0006198768,0.0003491018,0.00032707813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007283947,0.000096419026,0.97531974,0.000051894654,0.00037303873,0.00038541228,0.000088135464,0.002893102,0.007861293,0.0002765911,0.0015774732,0.010348465],"study_design_scores_gemma":[0.000016632688,0.00009451852,0.9915249,0.000007633206,0.00007755449,0.00019150654,0.00008447839,0.004312048,0.0016979545,0.000080797945,0.0019037973,0.000008090593],"about_ca_topic_score_codex":0.0041036126,"about_ca_topic_score_gemma":0.0052020587,"teacher_disagreement_score":0.0041036126,"about_ca_system_score_codex":0.00031020652,"about_ca_system_score_gemma":0.00026639152,"threshold_uncertainty_score":0.0085532665},"labels":[],"label_agreement":null},{"id":"W4392821468","doi":"10.3847/1538-4357/ad2268","title":"An Extremely Young Protostellar Core, MMS 1/OMC-3: Episodic Mass Ejection History Traced by the Micro SiO Jet","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astronomy; Astrophysics; Jet (fluid); Core (optical fiber); Protostar; Star formation; Stars; Optics; Mechanics","score_opus":0.01694051495998814,"score_gpt":0.24260031486275227,"score_spread":0.22565979990276414,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392821468","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994198,0.000020389141,0.00007908828,0.000009146545,0.0000011078624,0.0000034253942,0.00007939101,0.000012698659,0.00037504407],"genre_scores_gemma":[0.99942774,0.000009793357,0.00024217687,0.000014549665,0.0000029480582,0.0000021970143,0.00020199969,0.0000038642106,0.000094679504],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995744,0.0000023313312,0.000001550264,0.000012578405,0.000011003112,0.000015126351],"domain_scores_gemma":[0.99988425,0.0000074028053,0.00003542455,0.000010864393,0.0000098547325,0.000052143714],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000111935056,0.00017840137,0.00020913799,0.00034059378,0.00045187154,0.00030745685,0.00024522658,0.00025622523,0.00044806505],"category_scores_gemma":[0.00014483352,0.00012871835,0.00015243555,0.00020866234,0.00018001274,0.00011365129,0.0003477973,0.00026697657,0.00013854323],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003512253,0.00015603969,0.7837159,0.000032097625,0.00006708541,0.0038745757,0.000610258,0.0010940235,0.20200238,0.00030697146,0.0005925613,0.0071968953],"study_design_scores_gemma":[0.00000977517,0.000085438114,0.9936673,0.0000046535984,0.000011017006,0.00047822503,0.000106649866,0.0017327913,0.0032011108,0.000057743262,0.0006410964,0.0000041919493],"about_ca_topic_score_codex":0.0044181496,"about_ca_topic_score_gemma":0.01021736,"teacher_disagreement_score":0.0044181496,"about_ca_system_score_codex":0.00039657237,"about_ca_system_score_gemma":0.00011948129,"threshold_uncertainty_score":0.008784831},"labels":[],"label_agreement":null},{"id":"W4392822241","doi":"10.3847/1538-4357/ad4ed2","title":"Chemical Cartography with APOGEE: Two-process Parameters and Residual Abundances for 288,789 Stars from Data Release 17","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ministerio de Ciencia e Innovación; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Agencia Estatal de Investigación; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Stars; Residual; Process (computing); Cartography; Geography; Mathematics; Astrophysics; Geodesy; Physics; Computer science; Algorithm","score_opus":0.02831305198510448,"score_gpt":0.3158406585934046,"score_spread":0.2875276066083001,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392822241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8765451,0.00014633463,0.0047815186,0.00014346307,0.000026459382,0.00005128996,0.10657774,0.005205632,0.0065225633],"genre_scores_gemma":[0.73577684,0.00014058228,0.011808336,0.00008536111,0.000036154408,0.000100675745,0.24446216,0.001382771,0.006207054],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998242,0.000016897358,0.000015265858,0.000063210384,0.000060559978,0.000019934787],"domain_scores_gemma":[0.99899715,0.00017451135,0.00019624003,0.00035091327,0.00020365413,0.000077556084],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042098074,0.00035773104,0.00033576266,0.0017690775,0.00019880764,0.0005597427,0.00045789435,0.00024276949,0.0069158925],"category_scores_gemma":[0.001337803,0.00019059078,0.0004254707,0.0016256728,0.00012916062,0.00031589405,0.00045490722,0.00029234478,0.004883359],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00037518216,0.00012457275,0.8516784,0.00012123711,0.00017895518,0.00030406108,0.00027170294,0.013810252,0.006586314,0.0010849617,0.05876033,0.06670405],"study_design_scores_gemma":[0.00012715763,0.000060478174,0.9060056,0.000017078706,0.000045485704,0.00018894592,0.00012230355,0.026021514,0.004237626,0.00077990495,0.06236231,0.000031627085],"about_ca_topic_score_codex":0.019662967,"about_ca_topic_score_gemma":0.022922076,"teacher_disagreement_score":0.019662967,"about_ca_system_score_codex":0.00038438383,"about_ca_system_score_gemma":0.0003231409,"threshold_uncertainty_score":0.03909707},"labels":[],"label_agreement":null},{"id":"W4392911515","doi":"10.3847/1538-4357/ad1328","title":"Quaia, the Gaia-unWISE Quasar Catalog: An All-sky Spectroscopic Quasar Sample","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":60,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Research Council; University of California, Los Angeles; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; California Institute of Technology; European Space Agency; Flatiron Health; York University","keywords":"Quasar; Physics; Redshift; Astrophysics; Sky; Observatory; Astronomy; Photometric redshift; Galaxy","score_opus":0.013187826029646521,"score_gpt":0.25167531318209735,"score_spread":0.23848748715245083,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392911515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.77876556,0.0010540424,0.028292788,0.000502426,0.00013999129,0.0012427765,0.16788636,0.0038818754,0.01823409],"genre_scores_gemma":[0.6682852,0.000436359,0.038806837,0.00042180784,0.0002540084,0.0011916384,0.28012684,0.0005832133,0.009894092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99920183,0.00011083087,0.00006574633,0.00021242857,0.00032738072,0.00008187329],"domain_scores_gemma":[0.9960147,0.0003307294,0.00058558036,0.0011808203,0.0013307945,0.00055738515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017720626,0.00033504525,0.00051699346,0.0046188976,0.00072945224,0.0012980032,0.0010113453,0.00027118978,0.0060024294],"category_scores_gemma":[0.005279641,0.00028274162,0.00041940215,0.0027876839,0.00029305555,0.0009629793,0.0019435309,0.00051357696,0.0030952678],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039843842,0.0004897288,0.6307021,0.0003585277,0.00027954805,0.00046182168,0.0011072052,0.003298293,0.020657755,0.007047859,0.11693959,0.21825911],"study_design_scores_gemma":[0.00014273857,0.0001434021,0.8594725,0.0000514783,0.00009852245,0.00044759488,0.0002584541,0.010054409,0.0028654365,0.001556846,0.12485131,0.00005722574],"about_ca_topic_score_codex":0.013986749,"about_ca_topic_score_gemma":0.017452236,"teacher_disagreement_score":0.013986749,"about_ca_system_score_codex":0.00041922092,"about_ca_system_score_gemma":0.0010869763,"threshold_uncertainty_score":0.027810633},"labels":[],"label_agreement":null},{"id":"W4392912587","doi":"10.3847/1538-4357/ad2704","title":"ULTRASAT: A Wide-field Time-domain UV Space Telescope","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":102,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"","keywords":"Physics; Neutron star; Astronomy; Astrophysics; Supernova; Spitzer Space Telescope; Sky; Gravitational wave; Observatory; Telescope; Galaxy; Light curve; Gamma-ray burst","score_opus":0.006131357616654438,"score_gpt":0.22294378713112614,"score_spread":0.21681242951447172,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392912587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.32079226,0.0019420706,0.18464594,0.0026660783,0.0020582143,0.001332365,0.12609217,0.116852425,0.2436185],"genre_scores_gemma":[0.5578793,0.00040918676,0.22013883,0.0019519933,0.00080484984,0.0006900162,0.16499756,0.003383757,0.049744483],"study_design_codex":"not_applicable","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9991227,0.00009105568,0.000022937316,0.00023183816,0.0003763378,0.00015511946],"domain_scores_gemma":[0.9991109,0.00006588407,0.000098171855,0.00017951366,0.00024736434,0.00029818405],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001133528,0.0006571722,0.00051938335,0.0011179323,0.00088962476,0.001195983,0.0011198343,0.00055163703,0.016031155],"category_scores_gemma":[0.000981544,0.00036849914,0.00051079877,0.0008509528,0.00043979412,0.0012493072,0.0015701724,0.0010315115,0.0083748],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0032676184,0.00074738916,0.07050588,0.00022286526,0.00027143196,0.00054680917,0.0005761197,0.0042613447,0.11508231,0.011142004,0.5253217,0.26805457],"study_design_scores_gemma":[0.0014949057,0.0014742988,0.11137426,0.00011788626,0.00018841424,0.0009007276,0.00034972528,0.072850645,0.040759,0.010385822,0.75984156,0.00026268171],"about_ca_topic_score_codex":0.004178812,"about_ca_topic_score_gemma":0.006235214,"teacher_disagreement_score":0.016031155,"about_ca_system_score_codex":0.00049863994,"about_ca_system_score_gemma":0.00092197413,"threshold_uncertainty_score":0.053629518},"labels":[],"label_agreement":null},{"id":"W4392912721","doi":"10.3847/1538-4357/ad1ee4","title":"The Cosmos in Its Infancy: JADES Galaxy Candidates at z &gt; 8 in GOODS-S and GOODS-N","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":137,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Manitoba","funders":"Astrophysics Division; European Research Council; ARC Centre of Excellence for All-Sky Astrophysics; National Science Foundation; Fondation Merac; University of California, Santa Cruz; National Research Foundation; Science and Technology Facilities Council; European Commission; Johns Hopkins University; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; Space Telescope Science Institute","keywords":"Physics; Galaxy; Redshift; Reionization; James Webb Space Telescope; Astronomy; Astrophysics; Cosmic variance; Hubble Ultra-Deep Field; Photometric redshift; Stars; Advanced Camera for Surveys; Sky; Galaxy formation and evolution; Hubble space telescope; Hubble Deep Field","score_opus":0.006522350670558213,"score_gpt":0.2241226551252259,"score_spread":0.2176003044546677,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392912721","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955532,0.00041877906,0.00018337951,0.000094841,0.000011575626,0.000008121031,0.00086724845,0.000027410128,0.0028353566],"genre_scores_gemma":[0.99733835,0.00015594097,0.0002450322,0.00003759328,0.000016039707,0.0000065842837,0.001656809,0.000012951007,0.0005306756],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997093,0.000045977296,0.000027790691,0.000071703456,0.00008232665,0.000062844345],"domain_scores_gemma":[0.9976877,0.00030772758,0.00090975506,0.0003444716,0.00022073826,0.0005296792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009117481,0.00020008862,0.00020972587,0.0032759348,0.00046691147,0.0010184592,0.0003177347,0.000173541,0.0018521793],"category_scores_gemma":[0.001612193,0.00013198382,0.00017784735,0.0019933765,0.00041123628,0.0005023396,0.00092669996,0.00016039098,0.00059419865],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006880752,0.0000109233,0.9920757,0.000013115612,0.000021695792,0.00017455424,0.00031494137,0.000043545526,0.0010512843,0.00021305407,0.0009598246,0.0050525498],"study_design_scores_gemma":[0.0000030243964,0.000014454163,0.9965797,0.000014246203,0.000011781965,0.000234528,0.00029741589,0.00008035595,0.00022061742,0.0000633633,0.0024782047,0.0000022718857],"about_ca_topic_score_codex":0.0030105966,"about_ca_topic_score_gemma":0.008265037,"teacher_disagreement_score":0.0032759348,"about_ca_system_score_codex":0.00024711338,"about_ca_system_score_gemma":0.00020099862,"threshold_uncertainty_score":0.006196201},"labels":[],"label_agreement":null},{"id":"W4392917803","doi":"10.3847/1538-4357/ad226e","title":"X-Ray Polarization of the Black Hole X-Ray Binary 4U 1630–47 Challenges the Standard Thin Accretion Disk Scenario","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Goddard Space Flight Center; Istituto Nazionale di Fisica Nucleare; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Grantová Agentura České Republiky; Marshall Space Flight Center; Akademie Věd České Republiky; National Aeronautics and Space Administration; Ministerstvo Školství, Mládeže a Tělovýchovy; European Space Agency; Deutsche Forschungsgemeinschaft","keywords":"Physics; Astrophysics; Polarization (electrochemistry); Accretion disc; Accretion (finance); X-ray binary; Binary number; X-ray; Black hole (networking); Polarimetry; Astronomy; Scattering; Neutron star; Optics","score_opus":0.015072688984568794,"score_gpt":0.23801456354685704,"score_spread":0.22294187456228826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392917803","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984511,0.0001633679,0.00060929894,0.00007796735,0.000008200506,0.0000018261229,0.000033675147,0.000011833339,0.00064269995],"genre_scores_gemma":[0.9996294,0.00005612526,0.00019563876,0.000019215478,0.000012092025,9.808547e-7,0.00004496157,0.000002370923,0.000039378865],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997981,0.000051650404,0.0000118009575,0.00005069813,0.000053325908,0.000034433673],"domain_scores_gemma":[0.9989555,0.00027337373,0.0004937946,0.00012525906,0.000052508025,0.00009951879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008644637,0.00034349886,0.00048441533,0.0005594936,0.00051950436,0.0015191516,0.00038161047,0.00063642865,0.0011056355],"category_scores_gemma":[0.0019144608,0.00019528961,0.00017666696,0.00029772418,0.0011693297,0.00061083946,0.0009650555,0.00048370243,0.0002628273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014916869,0.000117132375,0.691331,0.00022769134,0.00026000215,0.0025524758,0.0006115389,0.006117751,0.269246,0.009261976,0.00056810735,0.018214649],"study_design_scores_gemma":[0.000096114185,0.0005286361,0.9201506,0.00010027689,0.00015197649,0.0028312816,0.0010324044,0.022441609,0.03633174,0.014068678,0.0022234602,0.00004334966],"about_ca_topic_score_codex":0.00036365318,"about_ca_topic_score_gemma":0.00025633126,"teacher_disagreement_score":0.0015191516,"about_ca_system_score_codex":0.00020515513,"about_ca_system_score_gemma":0.00013771425,"threshold_uncertainty_score":0.004571736},"labels":[],"label_agreement":null},{"id":"W4392952377","doi":"10.3847/1538-4357/ad2350","title":"Circumgalactic Environments Around Distant Quasars 3C 9 and 4C 05.84","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"NASA Exoplanet Science Institute; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Quasar; Astrophysics; Galaxy; Astronomy; Halo; Dark matter; Virial mass; Star formation","score_opus":0.007279948127435411,"score_gpt":0.2117510516264063,"score_spread":0.2044711034989709,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4392952377","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995214,0.00002300346,0.00002708124,0.000004753293,6.5303544e-7,0.0000015031098,0.000079596946,0.0000041729886,0.00033789157],"genre_scores_gemma":[0.99960023,0.00001628025,0.00007662533,0.00000870492,0.0000017027264,0.0000016681455,0.00020025384,0.0000014273794,0.000093101735],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999199,0.0000072299636,0.0000029067578,0.000024744413,0.00001932937,0.000025918818],"domain_scores_gemma":[0.99966383,0.00002392174,0.00015381133,0.000021611924,0.000041675557,0.000095033545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012278388,0.00015810753,0.0001958115,0.0008509978,0.0005753499,0.00050756906,0.00021196074,0.00018516272,0.0010527505],"category_scores_gemma":[0.00024889034,0.00010788988,0.000106539854,0.00042510967,0.00031710282,0.00018291535,0.00063428475,0.0002148978,0.0001552295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022989174,0.00010555568,0.9434614,0.000019967254,0.0000774702,0.00050746807,0.00078068126,0.0005728978,0.048179843,0.00026738347,0.0003533694,0.0054440964],"study_design_scores_gemma":[0.0000029571354,0.000018403916,0.99889475,0.0000020026102,0.0000072852267,0.00005894793,0.00017146705,0.00012587063,0.00049797504,0.000017794888,0.00020021884,0.0000023477953],"about_ca_topic_score_codex":0.018921537,"about_ca_topic_score_gemma":0.023954837,"teacher_disagreement_score":0.018921537,"about_ca_system_score_codex":0.00041406875,"about_ca_system_score_gemma":0.00013128256,"threshold_uncertainty_score":0.03762275},"labels":[],"label_agreement":null},{"id":"W4393006543","doi":"10.3847/1538-4357/ad20d3","title":"Recognizing Blazars Using Radio Morphology from the VLA Sky Survey","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Argonne National Laboratory; Planetary Science Division; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Office of Science; Max-Planck-Institut für Astronomie; Chinese Academy of Sciences; High Energy Physics; Deutsche Forschungsgemeinschaft; Gordon and Betty Moore Foundation; Queen's University Belfast; National Aeronautics and Space Administration; University College London; National Energy Research Scientific Computing Center; Space Telescope Science Institute; University of California, Los Angeles; University of Portsmouth; Los Alamos National Laboratory; Johns Hopkins University; University of Chicago; SLAC National Accelerator Laboratory; Queen's University; Ohio State University; Eötvös Loránd Tudományegyetem; California Institute of Technology; Smithsonian Institution; U.S. Department of Energy; University of Sussex; National Central University; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; Financiadora de Estudos e Projetos; University of Pennsylvania; Durham University; Fermilab; National Science Foundation","keywords":"Blazar; Sky; Physics; Astrophysics; Line-of-sight; Astronomy; Radio galaxy; Active galactic nucleus; Galaxy; Gamma ray","score_opus":0.02845496627634335,"score_gpt":0.2568648743341696,"score_spread":0.22840990805782624,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393006543","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97406864,0.00029780495,0.010168372,0.00008424684,0.000018257053,0.00011670665,0.007641283,0.0016302507,0.005974469],"genre_scores_gemma":[0.933568,0.0002910459,0.027248021,0.000055752098,0.000045107638,0.000055034136,0.036407094,0.00015022019,0.002179792],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997087,0.000023866072,0.000034123706,0.000071148745,0.00011673751,0.000045371424],"domain_scores_gemma":[0.9983816,0.00019689402,0.0005879431,0.00026765175,0.00039904093,0.00016685447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004245639,0.00042478906,0.00027102564,0.005587026,0.00029684303,0.0014280084,0.00036778304,0.00028254947,0.0024626532],"category_scores_gemma":[0.0017087237,0.00016885567,0.00028150593,0.0024849665,0.00014081594,0.00041055356,0.00049909716,0.00015512016,0.0020460063],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012025691,0.000056269837,0.9305809,0.000061294835,0.000057701993,0.00022922987,0.000103080485,0.0012950557,0.010925199,0.0002526767,0.0045648497,0.051753603],"study_design_scores_gemma":[0.000015701877,0.00004164627,0.98365015,0.00001945391,0.00004568102,0.00029963933,0.00011945764,0.00775316,0.0032432773,0.0001809682,0.0046183844,0.00001240538],"about_ca_topic_score_codex":0.005591725,"about_ca_topic_score_gemma":0.009555142,"teacher_disagreement_score":0.005591725,"about_ca_system_score_codex":0.0002213153,"about_ca_system_score_gemma":0.00029639958,"threshold_uncertainty_score":0.011118352},"labels":[],"label_agreement":null},{"id":"W4393006605","doi":"10.3847/1538-4357/ad2516","title":"First Determination in the Extended Corona of the 2D Thermal Evolution of a Current Sheet after a Solar Eruption","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Key Research and Development Program of China; National Natural Science Foundation of China; Bundesministerium für Wirtschaft und Energie; Ministry of Science and Technology of the People's Republic of China; Chinese Academy of Sciences; National Aeronautics and Space Administration","keywords":"Physics; Current sheet; Corona (planetary geology); Astronomy; Astrophysics; Thermal; Current (fluid); Coronal mass ejection; Solar flare; Solar physics; Astrobiology; Solar wind; Plasma; Magnetohydrodynamics; Meteorology; Nuclear physics","score_opus":0.007288460621219778,"score_gpt":0.24391237720430353,"score_spread":0.23662391658308377,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393006605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99297225,0.00027951188,0.0026234498,0.000041339146,0.000017596603,0.000017132743,0.00061358087,0.00022726128,0.0032078591],"genre_scores_gemma":[0.9978569,0.00006575885,0.001291312,0.000009684623,0.00002069336,0.000005693247,0.00045542157,0.00002259118,0.00027189462],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999734,0.0000024429828,8.116562e-7,0.000009311139,0.0000063930047,0.0000075172643],"domain_scores_gemma":[0.9998803,0.000016407965,0.000027141754,0.000019756086,0.00002389937,0.000032323576],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007777144,0.00017958773,0.00016531022,0.0006030986,0.00014640532,0.00047543534,0.00015176102,0.0002442801,0.0010636436],"category_scores_gemma":[0.00022238371,0.00014716154,0.0002490401,0.0002974246,0.00014656078,0.00019501663,0.00024445646,0.0001907244,0.00020507531],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0013406501,0.00031066677,0.35009053,0.00029807288,0.00051625434,0.004119161,0.0012212627,0.018045291,0.5415248,0.0015230384,0.0035115327,0.07749875],"study_design_scores_gemma":[0.000016663238,0.00011673073,0.97024363,0.000010459239,0.000046871126,0.0004289278,0.00010936688,0.0227669,0.004106998,0.00026963445,0.0018676054,0.000016178683],"about_ca_topic_score_codex":0.0009930572,"about_ca_topic_score_gemma":0.0013341568,"teacher_disagreement_score":0.0010636436,"about_ca_system_score_codex":0.00012001442,"about_ca_system_score_gemma":0.000081692,"threshold_uncertainty_score":0.0035582185},"labels":[],"label_agreement":null},{"id":"W4393055218","doi":"10.3847/1538-4357/ad1bf3","title":"Outflows Driven from a Magnetic Pseudodisk","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astronomy; Astrophysics","score_opus":0.007993155459630027,"score_gpt":0.23051204173822878,"score_spread":0.22251888627859875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393055218","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976654,0.000020735275,0.0010548299,0.00004114286,0.000014499666,0.000008660755,0.000072227944,0.000046585723,0.0010758269],"genre_scores_gemma":[0.9993457,0.000011079361,0.00035119223,0.0000139845115,0.0000037285786,0.0000028412126,0.00007999927,0.0000071055615,0.00018442706],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999577,0.000005625251,0.0000021710475,0.000008119853,0.000007796315,0.00001873318],"domain_scores_gemma":[0.99980146,0.00003302407,0.000039939052,0.000013379833,0.000019921144,0.000092375805],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010855488,0.00020882594,0.0002384237,0.00015064252,0.00041784343,0.0006489593,0.0003982594,0.00036719622,0.0014311513],"category_scores_gemma":[0.00040977797,0.00014024053,0.00036253995,0.00010393506,0.00044010632,0.00031995124,0.0004756557,0.00045866147,0.000100223675],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076848496,0.00048534092,0.072966896,0.000098002296,0.00013025386,0.0022096483,0.0002983519,0.83424675,0.07577517,0.006705102,0.0012588209,0.005057207],"study_design_scores_gemma":[0.00013348661,0.00015859486,0.024049886,0.000008283106,0.000012210935,0.00012633594,0.00009901857,0.9702158,0.003253037,0.0014679496,0.00046019096,0.0000151399345],"about_ca_topic_score_codex":0.0038401645,"about_ca_topic_score_gemma":0.0017223506,"teacher_disagreement_score":0.0038401645,"about_ca_system_score_codex":0.00044252185,"about_ca_system_score_gemma":0.00029629533,"threshold_uncertainty_score":0.007635653},"labels":[],"label_agreement":null},{"id":"W4393088159","doi":"10.3847/1538-4357/ad28c1","title":"The ALMaQUEST Survey. XIII. Understanding Radial Trends in Star Formation Quenching via the Relative Roles of Gas Availability and Star Formation Efficiency","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"","keywords":"Physics; Star (game theory); Star formation; Astrophysics; Quenching (fluorescence); Intergalactic star; Astronomy; Stars; Fluorescence; Optics","score_opus":0.0230974589546972,"score_gpt":0.2608612456302108,"score_spread":0.2377637866755136,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393088159","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8581445,0.0019703025,0.00056607777,0.001072051,0.00008778548,0.000063372405,0.11456641,0.0002847748,0.02324475],"genre_scores_gemma":[0.8944327,0.0005718451,0.0012007931,0.000512668,0.0001590313,0.00008370009,0.09432903,0.00007709505,0.00863308],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970007,0.000059394748,0.00001993923,0.0000936875,0.00006618485,0.000060882165],"domain_scores_gemma":[0.9986965,0.00010788538,0.0005763061,0.000089892994,0.00031143005,0.00021797312],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005086595,0.00014256229,0.00017575664,0.0016872212,0.00028448403,0.00080128486,0.0005178255,0.00023002527,0.0058450596],"category_scores_gemma":[0.0010795117,0.000075506905,0.00022139822,0.0018133353,0.00010876221,0.00047379467,0.00048360793,0.0002797249,0.0027336862],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000075314805,0.000031503554,0.97038907,0.00004325893,0.000047170368,0.00007295654,0.00012377421,0.00009375411,0.0009185193,0.0003746288,0.01507785,0.01275211],"study_design_scores_gemma":[0.000007767889,0.000019007975,0.9835096,0.000010520001,0.000009231338,0.000064890424,0.00014375949,0.00037611037,0.00018745105,0.00009076823,0.015577467,0.0000034356144],"about_ca_topic_score_codex":0.020996116,"about_ca_topic_score_gemma":0.048542637,"teacher_disagreement_score":0.020996116,"about_ca_system_score_codex":0.00038074524,"about_ca_system_score_gemma":0.00026623867,"threshold_uncertainty_score":0.04174781},"labels":[],"label_agreement":null},{"id":"W4393096440","doi":"10.3847/1538-4357/ad2687","title":"Limits on Optical Counterparts to the Repeating Fast Radio Burst 20180916B from High-speed Imaging with Gemini-North/‘Alopeke","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; McGill University","funders":"Fondo Nacional de Desarrollo Científico y Tecnológico; Division of Astronomical Sciences","keywords":"Physics; Fast radio burst; Astrophysics; Pulsar; Astronomy; Millisecond pulsar; Optical telescope; Telescope; Neutron star","score_opus":0.009579328528137096,"score_gpt":0.28344114508092866,"score_spread":0.27386181655279157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393096440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99629325,0.00014377122,0.00040769047,0.0000574067,0.000009779584,0.0000057107222,0.00037013143,0.000044564673,0.0026677777],"genre_scores_gemma":[0.99632794,0.00007778508,0.0015364559,0.00006352123,0.000023481325,0.000011248211,0.0014233745,0.000020394002,0.0005157764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983585,0.00001040144,0.000010373683,0.00005302547,0.000050090162,0.000040313458],"domain_scores_gemma":[0.9990079,0.00010983856,0.0004495057,0.00013869637,0.00011984126,0.00017432426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040130998,0.00025393016,0.00020937341,0.0007416914,0.0003182959,0.00054183934,0.00035014038,0.00040555504,0.0019395004],"category_scores_gemma":[0.0008179554,0.0002946359,0.00018751042,0.00036833988,0.00021900792,0.0003798174,0.00059583,0.00030043843,0.0004129717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039704106,0.000077022574,0.85791934,0.00006675558,0.000104154504,0.0005293919,0.00037884677,0.000367434,0.12293777,0.00018807284,0.0013509294,0.015683368],"study_design_scores_gemma":[0.00000923489,0.00005281018,0.99384105,0.000011542236,0.000022757651,0.0002978205,0.00007260944,0.00042248244,0.003103454,0.000043839213,0.0021149523,0.0000075234875],"about_ca_topic_score_codex":0.0023745392,"about_ca_topic_score_gemma":0.010311045,"teacher_disagreement_score":0.0023745392,"about_ca_system_score_codex":0.0002868333,"about_ca_system_score_gemma":0.00011365301,"threshold_uncertainty_score":0.0064882636},"labels":[],"label_agreement":null},{"id":"W4393103072","doi":"10.3847/1538-4357/ad220b","title":"Search for 10–1000 GeV Neutrinos from Gamma-Ray Bursts with IceCube","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Alliance de recherche numérique du Canada; Santen; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Fonds Wetenschappelijk Onderzoek; Nvidia; Marquette University","keywords":"Physics; Gamma-ray burst; Neutrino; Astrophysics; Baryon; Muon; Fermi Gamma-ray Space Telescope; Photosphere; Astronomy; Particle physics; Spectral line","score_opus":0.014042134520251298,"score_gpt":0.24989723153086052,"score_spread":0.23585509701060922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393103072","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9877008,0.00029370427,0.0026242468,0.00008284096,0.000020376368,0.00004379686,0.0049086427,0.0002015924,0.004124116],"genre_scores_gemma":[0.97716856,0.00017055353,0.007060351,0.0000788926,0.000027113412,0.00005790348,0.014474277,0.000056030527,0.0009063737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99936837,0.00013466501,0.000038913116,0.00015248866,0.000211561,0.000093932635],"domain_scores_gemma":[0.9979188,0.0010198756,0.00046489673,0.00022152442,0.00020703617,0.0001679344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014034329,0.00044373254,0.00054899754,0.0015190548,0.0004566518,0.0008986056,0.00041502801,0.00036381424,0.0018264254],"category_scores_gemma":[0.0018539326,0.00019055298,0.00051676884,0.0015838215,0.00022847137,0.0002932677,0.0006705266,0.00034388257,0.00040275216],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0035576506,0.00035614768,0.8809753,0.00016310885,0.00065757346,0.0008215715,0.00021931245,0.014689467,0.051993366,0.0015892214,0.0043427967,0.040634457],"study_design_scores_gemma":[0.00022631788,0.00077381707,0.85394835,0.00008169143,0.00037582358,0.0013572328,0.00043482403,0.060974523,0.06124847,0.0018702361,0.01865584,0.000052923224],"about_ca_topic_score_codex":0.0022996243,"about_ca_topic_score_gemma":0.003178905,"teacher_disagreement_score":0.0022996243,"about_ca_system_score_codex":0.00053339254,"about_ca_system_score_gemma":0.00044181355,"threshold_uncertainty_score":0.007422149},"labels":[],"label_agreement":null},{"id":"W4393181847","doi":"10.3847/1538-4357/ad250f","title":"Closing the Gap between Observed Low-mass Galaxy H i Kinematics and Cold Dark Matter Predictions","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Galaxy; Dark matter; Cold dark matter; Kinematics; Classical mechanics","score_opus":0.016348629522654548,"score_gpt":0.22641194930587122,"score_spread":0.21006331978321668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393181847","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92831695,0.0011856284,0.05450038,0.0016882769,0.00010881498,0.000013597833,0.00075671147,0.00089916575,0.012530521],"genre_scores_gemma":[0.9973489,0.00008399415,0.0019397392,0.00015980414,0.000028135455,0.0000033767326,0.00017917846,0.000049897284,0.0002068552],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995602,0.000101293124,0.000015006281,0.0001850144,0.00008638138,0.000052071468],"domain_scores_gemma":[0.9956736,0.001517065,0.0009968539,0.0010895189,0.00036383249,0.00035908824],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022461133,0.00067304075,0.00044469902,0.00063295435,0.00033645207,0.0023275942,0.0012129603,0.00048690612,0.0020904955],"category_scores_gemma":[0.007097416,0.00034714505,0.0003190764,0.0003204012,0.0014461853,0.0023192205,0.001484265,0.00095448975,0.0005156216],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005619834,0.00023336109,0.71264106,0.00034416214,0.0006571655,0.0003038611,0.00070268154,0.10205145,0.02435061,0.100645505,0.00569474,0.051813364],"study_design_scores_gemma":[0.000059605743,0.000085280284,0.43577528,0.00018071063,0.00010926412,0.00014106196,0.0005058406,0.40097705,0.014814618,0.14233221,0.0049126763,0.00010643621],"about_ca_topic_score_codex":0.00649482,"about_ca_topic_score_gemma":0.004290858,"teacher_disagreement_score":0.00649482,"about_ca_system_score_codex":0.001009901,"about_ca_system_score_gemma":0.00046315754,"threshold_uncertainty_score":0.012914062},"labels":[],"label_agreement":null},{"id":"W4393200913","doi":"10.3847/1538-4357/ad21fe","title":"The Atacama Cosmology Telescope: Millimeter Observations of a Population of Asteroids or: ACTeroids","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; McGill University","funders":"Comisión Nacional de Investigación Científica y Tecnológica; Natural Sciences and Engineering Research Council of Canada; University of Toronto; National Energy Research Scientific Computing Center; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Government of Ontario; Compute Canada; Princeton University; National Science Foundation","keywords":"Physics; Astronomy; Millimeter; Asteroid; Cosmology; Astrophysics; Population; Telescope; Astrobiology","score_opus":0.02403874515426946,"score_gpt":0.25714226101573134,"score_spread":0.23310351586146189,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393200913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99846965,0.00003412174,0.00012188866,0.00001758451,0.000001971314,0.0000029468279,0.0007179158,0.000010621046,0.00062324497],"genre_scores_gemma":[0.9979393,0.000027558646,0.00025890494,0.000012451757,0.000008284349,0.0000046509385,0.0015270711,0.000004626272,0.00021711021],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986887,0.00001675055,0.0000068907293,0.000040821178,0.000036754427,0.000029912331],"domain_scores_gemma":[0.99936134,0.000054280874,0.00023780605,0.00007506013,0.00010781212,0.00016372267],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039463356,0.00016444759,0.00020108871,0.00094273896,0.00030198166,0.0004201789,0.00021659216,0.0001798482,0.0008721254],"category_scores_gemma":[0.00052850606,0.0001293085,0.00013919579,0.00088559766,0.0001665268,0.00025414623,0.00040592847,0.00022730004,0.0002734405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000960393,0.000027194325,0.9892865,0.000010668022,0.00003375234,0.00005180996,0.0002365264,0.00018205722,0.0059090564,0.00007923481,0.0005246269,0.0035624565],"study_design_scores_gemma":[0.0000020897523,0.000007738101,0.99934465,7.499026e-7,0.0000032858836,0.000037382677,0.000036940673,0.00013181778,0.0001664773,0.000007894793,0.00025984333,0.0000010500892],"about_ca_topic_score_codex":0.008252441,"about_ca_topic_score_gemma":0.015669126,"teacher_disagreement_score":0.008252441,"about_ca_system_score_codex":0.00028176207,"about_ca_system_score_gemma":0.00016283886,"threshold_uncertainty_score":0.016408801},"labels":[],"label_agreement":null},{"id":"W4393232990","doi":"10.3847/1538-4357/ad2355","title":"A Unified Model for Bipolar Outflows from Young Stars: Kinematic and Mixing Structures in HH 30","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Astrophysics; Stars; Jet (fluid); Millimeter; Ionization; Magnetic field; Ion; Mechanics","score_opus":0.015396603864185237,"score_gpt":0.2541741883171868,"score_spread":0.23877758445300157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393232990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7739573,0.0009785149,0.15442689,0.0033801368,0.00013755972,0.00021509208,0.00073633983,0.0006475263,0.06552068],"genre_scores_gemma":[0.98687774,0.00021755132,0.005280894,0.00012565282,0.000083295985,0.00007604806,0.00015534648,0.00003454072,0.0071488763],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989486,0.000020928012,0.000005287949,0.000021814092,0.000022878201,0.00003428724],"domain_scores_gemma":[0.99978,0.000024442359,0.000047117475,0.000017305407,0.00004214912,0.00008904683],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032061143,0.00038566501,0.00043038375,0.00054589286,0.00081760663,0.00166965,0.0014190578,0.0013429685,0.0045588287],"category_scores_gemma":[0.00054447737,0.0002904102,0.0005707673,0.0002463444,0.0009900979,0.0019021282,0.00096970994,0.00055737357,0.00093791186],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013476553,0.00011087171,0.025996381,0.00005026373,0.000034924713,0.0012064032,0.0011861013,0.068029955,0.0055806134,0.8819408,0.00305837,0.012670542],"study_design_scores_gemma":[0.000117429154,0.00011580676,0.011182575,0.000030138863,0.000026095628,0.0004334679,0.0004764938,0.58526385,0.0003078233,0.3972189,0.0047809198,0.00004643897],"about_ca_topic_score_codex":0.005628776,"about_ca_topic_score_gemma":0.0025791484,"teacher_disagreement_score":0.005628776,"about_ca_system_score_codex":0.0009578523,"about_ca_system_score_gemma":0.000621519,"threshold_uncertainty_score":0.015250802},"labels":[],"label_agreement":null},{"id":"W4393248298","doi":"10.3847/1538-4357/ad5be6","title":"The Instability Mechanism of Compact Multiplanet Systems","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Instability; Mechanism (biology); Computer science; Physics; Mechanics","score_opus":0.014210016801307178,"score_gpt":0.2343604870113546,"score_spread":0.2201504702100474,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393248298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9799586,0.000119068805,0.016097203,0.00011820622,0.000011426328,0.000013336492,0.00004612242,0.00017559661,0.0034604338],"genre_scores_gemma":[0.9987752,0.000021294978,0.0009015069,0.00000765895,0.0000031292561,0.000005534198,0.000016031105,0.000008862722,0.00026081514],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998952,0.000022834223,0.0000062947547,0.000029068813,0.00003090425,0.000015725209],"domain_scores_gemma":[0.9994974,0.00012514525,0.00016626347,0.00009406131,0.000055174005,0.00006197195],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026696842,0.00023051594,0.00032353456,0.00051109464,0.0005869659,0.0007772952,0.00046060086,0.00037519762,0.0015721291],"category_scores_gemma":[0.0015257166,0.00013552401,0.00032736576,0.00024503705,0.00082015444,0.00092705415,0.0006787815,0.00031627313,0.00021825184],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021303106,0.00007703931,0.030377062,0.00007938888,0.00013829343,0.00062123564,0.0006952226,0.8663862,0.037640017,0.049351797,0.000903232,0.013517441],"study_design_scores_gemma":[0.000014813326,0.000047513073,0.0043964353,0.000005000072,0.000009745614,0.00013971142,0.000050730247,0.9843015,0.0024641184,0.008128712,0.00042801915,0.00001363697],"about_ca_topic_score_codex":0.002560167,"about_ca_topic_score_gemma":0.00083217066,"teacher_disagreement_score":0.002560167,"about_ca_system_score_codex":0.0006663272,"about_ca_system_score_gemma":0.00025935995,"threshold_uncertainty_score":0.005259335},"labels":[],"label_agreement":null},{"id":"W4393277474","doi":"10.3847/1538-4357/ad2077","title":"Super-Earth LHS3844b is Tidally Locked","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Natural Science Foundation of China; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astronomy; Astrobiology; Astrophysics; Earth (classical element)","score_opus":0.00985574663114124,"score_gpt":0.22513295560957367,"score_spread":0.21527720897843242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393277474","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998475,0.000031189607,0.00016431574,0.000032559677,0.0000036822164,0.0000011080656,0.00009910259,0.000032598575,0.0011604496],"genre_scores_gemma":[0.99954104,0.000011725764,0.00009403744,0.000018178234,0.0000025120905,0.0000011691255,0.0001553298,0.000008502987,0.00016755961],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994457,0.000004849368,0.0000026754385,0.000021154561,0.00001190983,0.000014875622],"domain_scores_gemma":[0.9997738,0.00002587019,0.0000749073,0.000035662782,0.00001599377,0.000073749834],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008613673,0.00016997432,0.00029665147,0.00035010217,0.00050974626,0.0005344641,0.00023300675,0.00027512718,0.0024305105],"category_scores_gemma":[0.0003073188,0.00013117831,0.0001869046,0.00032946287,0.0003849818,0.00028208838,0.00051273685,0.0002607218,0.0004886397],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00077176554,0.00013172362,0.61444527,0.0001489608,0.00013698683,0.0017754001,0.0005678171,0.010334442,0.34837532,0.004108606,0.0016841738,0.017519562],"study_design_scores_gemma":[0.0001421608,0.00042332817,0.8996051,0.00003399183,0.00007783976,0.0020268317,0.0009920207,0.049257535,0.02908377,0.0049400195,0.013358343,0.000059165377],"about_ca_topic_score_codex":0.0035885915,"about_ca_topic_score_gemma":0.0028334376,"teacher_disagreement_score":0.0035885915,"about_ca_system_score_codex":0.00044049372,"about_ca_system_score_gemma":0.00015567776,"threshold_uncertainty_score":0.008130848},"labels":[],"label_agreement":null},{"id":"W4393277574","doi":"10.3847/1538-4357/ad26e5","title":"Irradiated Disks May Settle into Staircases","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration","keywords":"Physics; Irradiation; Astronomy; Astrophysics; Nuclear physics","score_opus":0.010873873617658365,"score_gpt":0.26541077102187965,"score_spread":0.2545368974042213,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393277574","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9766525,0.00041092763,0.012843229,0.00033139266,0.00006724421,0.00004460958,0.00018019456,0.0005834029,0.008886476],"genre_scores_gemma":[0.99563783,0.00006272447,0.001458905,0.00011274685,0.000008306469,0.00001718647,0.00011420617,0.00007491366,0.0025132236],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998778,0.00001195592,0.00000580011,0.00003628874,0.000022287742,0.000045836445],"domain_scores_gemma":[0.999564,0.00008927075,0.000087933346,0.00010641326,0.000060813414,0.0000916481],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015306652,0.00026353262,0.0003584773,0.0003994788,0.0008185203,0.0017897119,0.00089050847,0.00090826856,0.006132553],"category_scores_gemma":[0.0011232615,0.00035879304,0.0004774969,0.00023651886,0.0007369944,0.0012062351,0.0010853703,0.00088740024,0.0008298142],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021074563,0.0008755713,0.080309,0.00042269626,0.0004780243,0.0068497956,0.004495735,0.42002508,0.2890757,0.13445032,0.012278482,0.04863214],"study_design_scores_gemma":[0.0003496343,0.0014658291,0.066074096,0.00013453339,0.00014073831,0.0016638748,0.0020820226,0.7384327,0.07911106,0.06955834,0.040761176,0.0002259903],"about_ca_topic_score_codex":0.0023597325,"about_ca_topic_score_gemma":0.0015846526,"teacher_disagreement_score":0.006132553,"about_ca_system_score_codex":0.00079338613,"about_ca_system_score_gemma":0.00024686236,"threshold_uncertainty_score":0.020515382},"labels":[],"label_agreement":null},{"id":"W4393307550","doi":"10.3847/1538-4357/ad1b5a","title":"Probing the Diversity of Type Ia Supernova Light Curves in the Open Supernova Catalog","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; University of Victoria; Herzberg Institute of Astrophysics","funders":"","keywords":"Physics; Supernova; Light curve; Astrophysics; Astronomy; Type II supernova","score_opus":0.022620913534368427,"score_gpt":0.2654244531961134,"score_spread":0.24280353966174498,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393307550","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99090075,0.00009311863,0.0060714693,0.000048506852,0.0000043199143,0.000008354136,0.0021783966,0.00009886889,0.00059620594],"genre_scores_gemma":[0.9910597,0.00006756886,0.0028996237,0.000013152947,0.000013123202,0.000008600072,0.00571701,0.000021777105,0.0001994386],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958843,0.00008302714,0.00003327174,0.000121392535,0.00011875555,0.0000551421],"domain_scores_gemma":[0.99753785,0.0007091224,0.0006690343,0.00043604613,0.00039615048,0.00025183163],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010398562,0.00027722734,0.00032977303,0.0033419046,0.00022213576,0.0009799952,0.0003127285,0.00025887846,0.0008333165],"category_scores_gemma":[0.0039386083,0.00012739217,0.0003370889,0.0019686944,0.0003102388,0.00076656847,0.00097893,0.0004173828,0.0002885294],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009441326,0.00007207835,0.9494004,0.000034401855,0.00012418866,0.000059694896,0.0001901924,0.012467152,0.0050943675,0.0012386459,0.0010046992,0.030219795],"study_design_scores_gemma":[0.000004367778,0.000028593016,0.93795836,0.000017377606,0.000018497783,0.000087645116,0.00025234246,0.057502802,0.0012064883,0.0016037631,0.0013001865,0.000019533325],"about_ca_topic_score_codex":0.005551199,"about_ca_topic_score_gemma":0.00937517,"teacher_disagreement_score":0.005551199,"about_ca_system_score_codex":0.000347168,"about_ca_system_score_gemma":0.0002538147,"threshold_uncertainty_score":0.011037767},"labels":[],"label_agreement":null},{"id":"W4393318308","doi":"10.3847/1538-4357/ad2930","title":"An Unusual Pulse Shape Change Event in PSR J1713+0747 Observed with the Green Bank Telescope and CHIME","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"McGill University; University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Office of Naval Research; McGill Space Institute; Jet Propulsion Laboratory; Goddard Space Flight Center; Magyar Tudományos Akadémia; University of Toronto; Natural Sciences and Engineering Research Council of Canada; Flatiron Health; Space Telescope Science Institute; National Aeronautics and Space Administration; Canada Foundation for Innovation; National Science Foundation; Compute Canada; McGill University; Smithsonian Astrophysical Observatory; Western Canada Research Grid; Canadian Institute for Advanced Research; Eötvös Loránd Tudományegyetem; California Institute of Technology","keywords":"Physics; Green Bank Telescope; Event (particle physics); Astronomy; Telescope; Astrophysics; Pulsar","score_opus":0.027778300767459355,"score_gpt":0.3193845469525023,"score_spread":0.29160624618504294,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393318308","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808466,0.000050775372,0.00020196808,0.00004486179,0.000010418276,0.000009938875,0.00025993306,0.00003584339,0.0013015892],"genre_scores_gemma":[0.9990582,0.00001949426,0.0002581862,0.000028781926,0.000009283846,0.000006886778,0.0003370239,0.000010832138,0.00027128868],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998721,0.0000075772973,0.0000035308783,0.000020468344,0.00005274022,0.000043574157],"domain_scores_gemma":[0.99965465,0.00003962227,0.00006971529,0.00004266518,0.0000727484,0.00012065369],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024093398,0.00016676643,0.00035262026,0.0009204149,0.000756039,0.00041043633,0.00038358496,0.00044928055,0.0008404876],"category_scores_gemma":[0.00044683748,0.00018722887,0.00024764077,0.0007810727,0.00044006627,0.00012582657,0.00051255315,0.00051292265,0.00024400633],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00085907395,0.00017166787,0.65219647,0.00008633147,0.0001962583,0.00627835,0.001436634,0.0008404017,0.31552523,0.0007060023,0.0026902703,0.01901331],"study_design_scores_gemma":[0.000010733949,0.000054797536,0.994073,0.000004927622,0.000016115917,0.00051304954,0.00015409368,0.00049259193,0.003469122,0.000040190916,0.0011602215,0.000011253964],"about_ca_topic_score_codex":0.024522236,"about_ca_topic_score_gemma":0.04695827,"teacher_disagreement_score":0.024522236,"about_ca_system_score_codex":0.00069650076,"about_ca_system_score_gemma":0.00048745013,"threshold_uncertainty_score":0.048759043},"labels":[],"label_agreement":null},{"id":"W4393318633","doi":"10.3847/1538-4357/ad2c90","title":"A Measurement of the Assembly of Milky Way Analogs at Redshifts 0.5 &lt; z &lt; 2 with Resolved Stellar Mass and Star Formation Rate Profiles","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Physics; Milky Way; Star formation; Redshift; Astrophysics; Star (game theory); Astronomy; Stellar mass; Stars; Galaxy","score_opus":0.01053503820736997,"score_gpt":0.2011080862936801,"score_spread":0.19057304808631012,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393318633","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998809,0.00003028785,0.00019405097,0.0000048077154,6.5463064e-7,0.0000030658714,0.0003772912,0.000023055321,0.0005579793],"genre_scores_gemma":[0.99906427,0.000010397607,0.00017785952,0.00000443024,0.0000013817858,0.0000022262507,0.00050888356,0.000004026597,0.0002265771],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999144,0.000006913068,0.000005299573,0.000030245792,0.000021217733,0.000022016728],"domain_scores_gemma":[0.9991748,0.00005836026,0.00037237286,0.00006350183,0.000096645694,0.00023438309],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017595466,0.00015895828,0.00011704718,0.0011435742,0.00015137038,0.0005111188,0.00022129799,0.00024375287,0.0013972915],"category_scores_gemma":[0.0006504321,0.00014849742,0.00020742256,0.00050980214,0.00017207272,0.00036816977,0.00042955822,0.0001662124,0.0004137089],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000109224566,0.00002148709,0.9676338,0.000010923764,0.000035268127,0.00008787403,0.00021732839,0.000236541,0.027584955,0.000118272925,0.00011119352,0.003833094],"study_design_scores_gemma":[6.1959463e-7,0.000009084434,0.9987921,7.022521e-7,0.0000032601042,0.000030105255,0.00002513556,0.000162455,0.00086886185,0.0000075213484,0.0000991178,0.0000010864958],"about_ca_topic_score_codex":0.0034444553,"about_ca_topic_score_gemma":0.004321554,"teacher_disagreement_score":0.0034444553,"about_ca_system_score_codex":0.00030595882,"about_ca_system_score_gemma":0.00006547532,"threshold_uncertainty_score":0.006848812},"labels":[],"label_agreement":null},{"id":"W4393318639","doi":"10.3847/1538-4357/ad25ff","title":"Helium-deficient ER UMa-type Dwarf Nova below the Period Minimum with a Hot Secondary","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Research Foundation of Korea","keywords":"Physics; Dwarf nova; Astrophysics; Nova (rocket); Helium; Period (music); Astronomy; White dwarf; Stars; Atomic physics","score_opus":0.01431857818987409,"score_gpt":0.23794708207881715,"score_spread":0.22362850388894306,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393318639","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977883,0.00017299854,0.00028178783,0.000019240948,0.000013095997,0.0000083911145,0.00017256352,0.000022020993,0.0015215874],"genre_scores_gemma":[0.9993418,0.000026374568,0.00017725285,0.00001623824,0.000009080535,0.0000023998325,0.0001926487,0.0000038361504,0.0002304116],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998685,0.0000050635567,0.000010193259,0.000046495617,0.000027236802,0.000042397776],"domain_scores_gemma":[0.999559,0.000021249549,0.00012782455,0.00003730579,0.000039265018,0.00021521376],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009671644,0.00030769847,0.00040780398,0.00082775805,0.0006438399,0.0005312144,0.00029609454,0.00035073422,0.0011862098],"category_scores_gemma":[0.0002723363,0.00018563699,0.00029890105,0.0004150621,0.00032136912,0.0002178317,0.0004884404,0.00035954636,0.00045175955],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00059619674,0.0001322415,0.8295415,0.000103895094,0.00009798857,0.025436837,0.00021829967,0.0002982926,0.13306949,0.0004174276,0.0006097565,0.009478083],"study_design_scores_gemma":[0.000015848316,0.0001678386,0.9485796,0.000013553586,0.000034029057,0.038217667,0.00020824304,0.00064166717,0.00951982,0.0001828248,0.002406791,0.000012085879],"about_ca_topic_score_codex":0.0015001956,"about_ca_topic_score_gemma":0.0017205954,"teacher_disagreement_score":0.0015001956,"about_ca_system_score_codex":0.00028994904,"about_ca_system_score_gemma":0.0001454971,"threshold_uncertainty_score":0.0039682984},"labels":[],"label_agreement":null},{"id":"W4393335225","doi":"10.3847/1538-4357/ad3c43","title":"JWST Photometric Time-delay and Magnification Measurements for the Triply Imaged Type Ia “SN H0pe” at z = 1.78","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; Goddard Space Flight Center; Stony Brook University; Max-Planck-Gesellschaft; Knut och Alice Wallenbergs Stiftelse; Science and Technology Facilities Council; Ministero dell’Istruzione, dell’Università e della Ricerca; California Institute of Technology; European Commission; Deutsche Forschungsgemeinschaft; European Science Foundation; Space Telescope Science Institute; Villum Fonden; Jet Propulsion Laboratory; Aspen Center for Physics; Javna Agencija za Raziskovalno Dejavnost RS; Nuclear Safety and Security Commission; Ministerio de Ciencia, Innovación y Universidades; United States-Israel Binational Science Foundation; United States - Israel Binational Agricultural Research and Development Fund; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; James Webb Space Telescope; Photometry (optics); Astrophysics; Supernova; Galaxy; Light curve; Magnification; Population; Hubble space telescope; Stars; Optics","score_opus":0.03007517065008409,"score_gpt":0.2776225747450234,"score_spread":0.2475474040949393,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393335225","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99008596,0.00008163399,0.0010121996,0.000029058985,0.000015062266,0.000009029266,0.00348273,0.00042116968,0.0048630387],"genre_scores_gemma":[0.9909713,0.000052526782,0.0021871314,0.00002348122,0.000016001763,0.000010179519,0.0055312347,0.00008477656,0.0011234541],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999145,0.0000027200376,0.000004577197,0.000026642789,0.000036758454,0.000014849095],"domain_scores_gemma":[0.9995802,0.00003348231,0.00012594117,0.00004189206,0.00010493596,0.00011348209],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018136016,0.00021690052,0.00012812432,0.001533777,0.00019502241,0.0002937375,0.0003147841,0.00022587932,0.0022790886],"category_scores_gemma":[0.00044696103,0.00016240637,0.00019940108,0.00066798035,0.000107864675,0.00030051664,0.000310232,0.00027255708,0.00074869185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00063192006,0.0002044236,0.626952,0.0000863591,0.00013657448,0.0004963331,0.00037395206,0.0020365836,0.32081923,0.0009836196,0.0074694394,0.039809514],"study_design_scores_gemma":[0.000006537369,0.000039851362,0.97886443,0.0000036854185,0.000018130824,0.00021739492,0.000026076212,0.0026394639,0.016607532,0.00006621956,0.0015004601,0.000010160378],"about_ca_topic_score_codex":0.0053669987,"about_ca_topic_score_gemma":0.0084720105,"teacher_disagreement_score":0.0053669987,"about_ca_system_score_codex":0.00033954758,"about_ca_system_score_gemma":0.000083914856,"threshold_uncertainty_score":0.010671556},"labels":[],"label_agreement":null},{"id":"W4393377580","doi":"10.3847/1538-4357/ad2c92","title":"A Relook at the Black Hole Binary Candidate J1328+2752 with VLBI","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Very-long-baseline interferometry; Astrophysics; Binary number; Black hole (networking); Physics; Computer science; Mathematics; Computer security","score_opus":0.005249164786505932,"score_gpt":0.2050061025743564,"score_spread":0.19975693778785045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393377580","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99506736,0.00013795562,0.0007280147,0.00013335931,0.00001794572,0.000021638414,0.0006849058,0.0001418854,0.0030668983],"genre_scores_gemma":[0.9953057,0.000032442804,0.0016719933,0.00008454349,0.00002268208,0.000011324422,0.0016213608,0.000021347523,0.0012286486],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999049,0.0000074651903,0.0000032405624,0.000024487084,0.000027782826,0.000032209624],"domain_scores_gemma":[0.9997837,0.000010690617,0.000044193468,0.00003070721,0.000033572072,0.000097146425],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002120804,0.00025683938,0.00022904766,0.0011230893,0.00050741545,0.00047890632,0.0003148672,0.00032028364,0.0020248024],"category_scores_gemma":[0.0002581233,0.00017637493,0.00021037256,0.00049075467,0.0001283989,0.0002172619,0.00048730496,0.00032753372,0.00061963813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00096494873,0.00052532344,0.62488,0.000096861586,0.00023246216,0.003845022,0.0007091619,0.0014535094,0.3190587,0.0007930075,0.005703248,0.041737784],"study_design_scores_gemma":[0.000027164742,0.00013803013,0.98546046,0.000011799212,0.00004820499,0.00050407107,0.00024235235,0.002539442,0.0052573294,0.00017712235,0.0055802977,0.000013717552],"about_ca_topic_score_codex":0.0060345717,"about_ca_topic_score_gemma":0.01744442,"teacher_disagreement_score":0.0060345717,"about_ca_system_score_codex":0.0004472227,"about_ca_system_score_gemma":0.00019402622,"threshold_uncertainty_score":0.011998892},"labels":[],"label_agreement":null},{"id":"W4393387399","doi":"10.3847/1538-4357/ad2513","title":"Optical- and UV-continuum Morphologies of Compact Radio Source Hosts","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Space Telescope Science Institute; Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; Jet Propulsion Laboratory; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Active galactic nucleus; Radio galaxy; Star formation; Galaxy; Redshift; Astronomy; X-shaped radio galaxy; Quasar","score_opus":0.007552392239312702,"score_gpt":0.21877179644437825,"score_spread":0.21121940420506555,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393387399","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994412,0.000062763844,0.00005582385,0.0000019584961,7.063178e-7,0.0000018034324,0.00014693786,0.000006210836,0.0002825188],"genre_scores_gemma":[0.999559,0.00002108392,0.00006306375,0.000002926181,0.0000020891823,0.0000013376058,0.00022254612,0.0000022325462,0.0001256978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999926,0.0000053637114,0.0000060389275,0.00002309099,0.000014509836,0.000024949963],"domain_scores_gemma":[0.9994398,0.000057840476,0.00021486758,0.00004881482,0.0000736144,0.00016516502],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013464181,0.00016475443,0.00013616092,0.0012971405,0.00017097562,0.00050949317,0.00018335207,0.00012715878,0.0016913007],"category_scores_gemma":[0.0004212407,0.00008816409,0.00010293306,0.00038717408,0.00021591832,0.00019275959,0.00030845066,0.000099559176,0.00038279095],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000102771206,0.000023503204,0.98114944,0.000010790341,0.00001648816,0.000226177,0.00016511804,0.00006918643,0.014280444,0.000032856424,0.00006429448,0.0038589113],"study_design_scores_gemma":[0.0000018966093,0.0000651294,0.99808204,0.0000022381366,0.000007731295,0.0006277689,0.00011925727,0.0001113325,0.0008120967,0.000015356612,0.00015354042,0.0000017431923],"about_ca_topic_score_codex":0.0012430423,"about_ca_topic_score_gemma":0.0015810685,"teacher_disagreement_score":0.0016913007,"about_ca_system_score_codex":0.00013658003,"about_ca_system_score_gemma":0.000041890962,"threshold_uncertainty_score":0.0056580305},"labels":[],"label_agreement":null},{"id":"W4393392919","doi":"10.3847/1538-4357/ad2941","title":"Testing EMRI Models for Quasi-periodic Eruptions with 3.5 yr of Monitoring eRO-QPE1","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Structural Health Monitoring Techniques","field":"Engineering","cited_by":43,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"Istituto Nazionale di Astrofisica; European Commission; Australian Government; Space Telescope Science Institute; Comunidad de Madrid; Agencia Estatal de Investigación; National Aeronautics and Space Administration","keywords":"Geology; Environmental science; Seismology","score_opus":0.037975949377373676,"score_gpt":0.29755133996115884,"score_spread":0.25957539058378515,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393392919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9912559,0.00012173261,0.006310977,0.00025115593,0.000016792155,0.000029811526,0.00082944514,0.00014268815,0.0010414929],"genre_scores_gemma":[0.9963995,0.000032517262,0.0020755024,0.00003890927,0.000019138291,0.000027257789,0.0010396006,0.000034374923,0.0003331384],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9991748,0.00025835895,0.000041001353,0.00033721564,0.00005083374,0.00013774795],"domain_scores_gemma":[0.99397635,0.0038064267,0.0010959958,0.00040922844,0.0003551624,0.00035679364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0043045473,0.00062884483,0.00053117337,0.0005411511,0.00033574586,0.0010636593,0.0019685004,0.001046032,0.0017840619],"category_scores_gemma":[0.008350498,0.00033423398,0.0011406211,0.00029842783,0.0004956642,0.0008802249,0.0008420624,0.00067703804,0.00037253503],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00076916086,0.00039231652,0.4909313,0.0001297907,0.00050571404,0.0005667784,0.0003317104,0.48355177,0.0040353374,0.004378828,0.0015186382,0.012888722],"study_design_scores_gemma":[0.000034970548,0.000097785756,0.03897862,0.000008386963,0.00004987839,0.000070257214,0.000072475385,0.95908695,0.0004696181,0.0007350744,0.00038354364,0.000012376134],"about_ca_topic_score_codex":0.019748483,"about_ca_topic_score_gemma":0.007545609,"teacher_disagreement_score":0.019748483,"about_ca_system_score_codex":0.0012306424,"about_ca_system_score_gemma":0.0005535212,"threshold_uncertainty_score":0.039267063},"labels":[],"label_agreement":null},{"id":"W4393393044","doi":"10.3847/1538-4357/ad2dfc","title":"COMAP Early Science. VIII. A Joint Stacking Analysis with eBOSS Quasars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Jet Propulsion Laboratory; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Norges Forskningsråd; University of Oxford; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Keck Institute for Space Studies; University of Toronto; Yale University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Ohio State University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; York University; University of Miami; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; National Science Foundation","keywords":"Stacking; Joint (building); Computer science; Computational biology; Engineering; Physics; Biology; Structural engineering","score_opus":0.016076543191890783,"score_gpt":0.28520556081626236,"score_spread":0.2691290176243716,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393393044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6331668,0.0011058731,0.053503517,0.0016542798,0.00034796944,0.00019537793,0.17072153,0.02039948,0.118905276],"genre_scores_gemma":[0.7660488,0.0005563641,0.052070357,0.00024386591,0.000397305,0.00012422024,0.14964119,0.0035107904,0.027407095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996032,0.00003189349,0.000013887374,0.00007542838,0.00015614419,0.00011942911],"domain_scores_gemma":[0.99861276,0.0001695609,0.0002080436,0.00038933437,0.00032303066,0.00029714228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00078654906,0.0006053633,0.0003255336,0.0035378593,0.00085317943,0.0020409885,0.0005367535,0.00024524482,0.02049896],"category_scores_gemma":[0.0020001116,0.00027475812,0.0006333378,0.0043312944,0.0002067814,0.00083799945,0.0015237493,0.0005510739,0.0072367364],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001044447,0.00023634605,0.38984483,0.00021205975,0.0005734007,0.0016226616,0.0013761309,0.0055313716,0.015221118,0.013808002,0.2007559,0.36977375],"study_design_scores_gemma":[0.000054880078,0.00009085576,0.74955845,0.00004903395,0.00021996774,0.00034044345,0.00075665244,0.017278269,0.0066534826,0.00992258,0.21501341,0.00006188992],"about_ca_topic_score_codex":0.012811905,"about_ca_topic_score_gemma":0.0108686015,"teacher_disagreement_score":0.02049896,"about_ca_system_score_codex":0.00038109656,"about_ca_system_score_gemma":0.00047875065,"threshold_uncertainty_score":0.06857586},"labels":[],"label_agreement":null},{"id":"W4393421739","doi":"10.3847/1538-4357/ad2267","title":"Ursa Major III/UNIONS 1: The Darkest Galaxy Ever Discovered?","year":2024,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":27,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"HORIZON EUROPE European Research Council; European Commission; National Science Foundation","keywords":"Physics; Galaxy; Milky Way; Velocity dispersion; Astrophysics","score_opus":0.010924067967469427,"score_gpt":0.23369780679174043,"score_spread":0.222773738824271,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393421739","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9152195,0.013065702,0.0017623304,0.0060454067,0.00046785834,0.000027897495,0.0051793274,0.001139514,0.0570925],"genre_scores_gemma":[0.97280926,0.002320432,0.0019082996,0.0010431211,0.00047026703,0.000010956738,0.0060460344,0.00015420218,0.015237508],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986017,0.000010814585,0.0000039954098,0.00005072768,0.00002337671,0.000050817016],"domain_scores_gemma":[0.9996457,0.000028570785,0.00007238028,0.000047742455,0.000038665523,0.00016704979],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024086691,0.0002717338,0.00028583032,0.0009823607,0.0008654786,0.0011507751,0.00037814135,0.00046705303,0.007411709],"category_scores_gemma":[0.0004708363,0.00018887433,0.00015531004,0.0006760043,0.00048009196,0.0009424768,0.0008603381,0.0005138634,0.0026889802],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009222369,0.00013594927,0.5656163,0.0004789894,0.00010351889,0.0025673823,0.0026590556,0.00031903066,0.026854832,0.017696394,0.14753188,0.23511444],"study_design_scores_gemma":[0.000034722354,0.00018441307,0.5472742,0.00023032312,0.00009611135,0.0034973535,0.0032000474,0.0006164848,0.006274965,0.009158472,0.42938757,0.000045336576],"about_ca_topic_score_codex":0.004492795,"about_ca_topic_score_gemma":0.0069824047,"teacher_disagreement_score":0.007411709,"about_ca_system_score_codex":0.00071132183,"about_ca_system_score_gemma":0.00026406156,"threshold_uncertainty_score":0.024794698},"labels":[],"label_agreement":null},{"id":"W4393716549","doi":"10.3847/1538-4357/ad25ed","title":"Stellar Metallicities and Gradients in the Isolated, Quenched Low-mass Galaxy Tucana","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Herzberg Institute of Astrophysics","funders":"NASA Headquarters; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Dwarf galaxy; Astronomy","score_opus":0.009299191851252369,"score_gpt":0.2213316952670375,"score_spread":0.21203250341578514,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393716549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981639,0.000056681376,0.00007748467,0.00003291538,0.0000023417185,0.0000039026054,0.00042516284,0.00003780582,0.0011998852],"genre_scores_gemma":[0.99907196,0.00001565181,0.00008658714,0.00001576893,0.0000024207334,0.0000031050774,0.00053536874,0.000008277167,0.00026093345],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981254,0.000007655456,0.0000043493487,0.00007937556,0.000030404597,0.00006573402],"domain_scores_gemma":[0.9993825,0.00004413922,0.000107591426,0.00006512302,0.00015914439,0.00024143423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021221796,0.00030728805,0.00041103564,0.0011594782,0.001347296,0.001585636,0.0009762085,0.00034390323,0.002385579],"category_scores_gemma":[0.0009065881,0.00017070016,0.00021494308,0.0009685161,0.0009445948,0.00031730635,0.00078023697,0.0003512517,0.00035939147],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000499211,0.00013519681,0.95089024,0.000032467662,0.00019749423,0.00020396788,0.00089396886,0.0033010358,0.027666662,0.0007882802,0.0015304079,0.013861234],"study_design_scores_gemma":[0.000014953516,0.0000202557,0.9943277,0.0000075875464,0.000042047828,0.000033578995,0.0004842018,0.0022552796,0.0015886793,0.00014609857,0.0010684509,0.000011050844],"about_ca_topic_score_codex":0.44953513,"about_ca_topic_score_gemma":0.40907004,"teacher_disagreement_score":0.44953513,"about_ca_system_score_codex":0.003583766,"about_ca_system_score_gemma":0.0008835761,"threshold_uncertainty_score":0.8938371},"labels":[],"label_agreement":null},{"id":"W4393901744","doi":"10.3847/1538-4357/ad283c","title":"Electromagnetic Signatures of Mirror Stars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Stars; Astronomy; Physics; Astrophysics","score_opus":0.007594163976385027,"score_gpt":0.22740738032313998,"score_spread":0.21981321634675496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4393901744","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9837104,0.00007760903,0.011359506,0.000032905635,0.0000061089945,0.0000051166353,0.0003267163,0.00015633888,0.0043254243],"genre_scores_gemma":[0.9984842,0.000011803761,0.0010980727,0.000008762554,0.00000197589,0.0000014510076,0.00015013826,0.000012386006,0.00023113057],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993145,0.0000123211,0.0000028646418,0.000025032372,0.000012707074,0.000015560781],"domain_scores_gemma":[0.99965894,0.00009623622,0.00008937916,0.000060953324,0.000047139274,0.000047318266],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020939218,0.00014669332,0.0001678631,0.0006348242,0.00019994959,0.00047137093,0.00019990308,0.00023728369,0.0015184995],"category_scores_gemma":[0.00064964156,0.00008157446,0.00012835544,0.00031115883,0.000215007,0.0002926253,0.00035763605,0.00017767363,0.00029636596],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083023723,0.000087020235,0.5666038,0.00019672295,0.00013575405,0.0010135695,0.000637349,0.027021468,0.30097663,0.050232694,0.0025784485,0.049686275],"study_design_scores_gemma":[0.0000564227,0.00025982328,0.65013844,0.000056227283,0.00005952001,0.0022321935,0.00045879712,0.1657175,0.12951691,0.040868282,0.010558248,0.000077652134],"about_ca_topic_score_codex":0.00024059859,"about_ca_topic_score_gemma":0.00025111376,"teacher_disagreement_score":0.0015184995,"about_ca_system_score_codex":0.00015373323,"about_ca_system_score_gemma":0.00004625677,"threshold_uncertainty_score":0.0050798655},"labels":[],"label_agreement":null},{"id":"W4394596522","doi":"10.3847/1538-4357/ad2261","title":"Interpretable Machine Learning for Finding Intermediate-mass Black Holes","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Mila - Quebec Artificial Intelligence Institute","funders":"HORIZON EUROPE European Research Council; HORIZON EUROPE Marie Sklodowska-Curie Actions; Canada Research Chairs; Schmidt Family Foundation","keywords":"Artificial intelligence; Computer science; Machine learning","score_opus":0.013967772504449964,"score_gpt":0.3250049917372193,"score_spread":0.31103721923276934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394596522","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.25230747,0.0006338228,0.74079716,0.0014671286,0.00009827095,0.00008618724,0.00021652698,0.001988239,0.0024051259],"genre_scores_gemma":[0.93595624,0.000072514726,0.062375892,0.00028526312,0.00007573454,0.000055272885,0.00036069422,0.00009488239,0.0007236119],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99912876,0.00041167173,0.000037790145,0.00018207834,0.00015445567,0.000085218606],"domain_scores_gemma":[0.9946278,0.003663954,0.000481818,0.00042514305,0.0005709133,0.00023039932],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0034210517,0.0008021983,0.0010691156,0.0012335723,0.00058017106,0.0012617307,0.0023512735,0.0016849595,0.0014815277],"category_scores_gemma":[0.012185457,0.00044281033,0.00077447126,0.00050133956,0.0015585605,0.0011252773,0.0013806492,0.001926401,0.00038483355],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001239237,0.0000898595,0.008237789,0.000060792067,0.000048760154,0.00012385966,0.00011601623,0.9421095,0.0010159382,0.008664377,0.0014362686,0.037972894],"study_design_scores_gemma":[0.0000041120834,0.000008690077,0.00020731827,0.000004461624,0.0000020156003,0.00000525089,0.000005775296,0.99318755,0.00018342173,0.0063156,0.00007390504,0.000001974588],"about_ca_topic_score_codex":0.0025711295,"about_ca_topic_score_gemma":0.0018727365,"teacher_disagreement_score":0.0034210517,"about_ca_system_score_codex":0.0010697998,"about_ca_system_score_gemma":0.0006270506,"threshold_uncertainty_score":0.018092453},"labels":[],"label_agreement":null},{"id":"W4394596614","doi":"10.3847/1538-4357/ad2a49","title":"SN 2022jox: An Extraordinarily Ordinary Type II SN with Flash Spectroscopy","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Saskatchewan","funders":"Heising-Simons Foundation; National Science Foundation","keywords":"Flash (photography); Spectroscopy; Type (biology); Materials science; Physics; Optics; Geology; Astronomy","score_opus":0.010023815676791394,"score_gpt":0.2478806375207102,"score_spread":0.23785682184391882,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394596614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99197197,0.00021810303,0.00061476824,0.00007346562,0.000044428118,0.00002428686,0.00066553615,0.00012391916,0.006263518],"genre_scores_gemma":[0.9931995,0.00010621819,0.00084804546,0.0001622166,0.0000619937,0.000014950316,0.0021174466,0.000037174923,0.003452408],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995923,0.0000022153663,0.0000024922144,0.000012991543,0.000009962006,0.000013023348],"domain_scores_gemma":[0.99992335,0.0000049990003,0.000012591191,0.000009429287,0.000008767647,0.000040757623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006573413,0.0005564576,0.00021322294,0.00044075982,0.000337311,0.00037909372,0.00019502128,0.0003736378,0.0031044479],"category_scores_gemma":[0.0001102379,0.00011441364,0.00012371622,0.00020484744,0.00012783534,0.00019863444,0.00040629567,0.00022112884,0.00075116067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001464484,0.0004513898,0.6403795,0.0002411731,0.00016125225,0.035797708,0.00040964113,0.0011167653,0.2561393,0.0022681702,0.016093243,0.045477413],"study_design_scores_gemma":[0.0000674843,0.0007815281,0.9104699,0.0000311042,0.000051875417,0.031569827,0.00036647517,0.0027865353,0.018690465,0.00082553894,0.034325168,0.00003405533],"about_ca_topic_score_codex":0.0011486034,"about_ca_topic_score_gemma":0.0022482781,"teacher_disagreement_score":0.0031044479,"about_ca_system_score_codex":0.000115740084,"about_ca_system_score_gemma":0.000053552325,"threshold_uncertainty_score":0.010385394},"labels":[],"label_agreement":null},{"id":"W4394686133","doi":"10.3847/1538-4357/ad2df7","title":"SN 2023ixf in Messier 101: The Twilight Years of the Progenitor as Seen by Pan-STARRS","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":31,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Charles E. Kaufman Foundation; Canada Research Chairs; National Aeronautics and Space Administration; University of Toronto; Villum Fonden; University of California Institute for Mexico and the United States; National Science Foundation","keywords":"Physics; Supernova; Photometry (optics); Red supergiant; Astrophysics; Stars; Limiting; Supergiant; Luminosity; Galaxy","score_opus":0.006009041199798741,"score_gpt":0.22944413285397935,"score_spread":0.2234350916541806,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394686133","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873704,0.00003423451,0.00015391763,0.000023281564,0.0000024507037,0.000004696866,0.00039904882,0.000030353302,0.00061503635],"genre_scores_gemma":[0.9983072,0.000024474319,0.00020996148,0.000014002725,0.0000047862877,0.0000034384798,0.0009810225,0.000008491186,0.0004465118],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996054,0.000002618616,0.0000029507862,0.000014172043,0.000010497414,0.000009142752],"domain_scores_gemma":[0.999838,0.000022658125,0.000058713787,0.000015617885,0.00001209245,0.00005284883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015073635,0.00018197353,0.0002020252,0.00056264905,0.00021140346,0.0002949768,0.00018822981,0.00033388747,0.002003118],"category_scores_gemma":[0.0003941724,0.00008773101,0.00026730206,0.00029921182,0.00013542727,0.00018927854,0.0002693068,0.00020348595,0.00044594496],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030077895,0.00003933726,0.96954465,0.000020514051,0.000055464054,0.0017531964,0.00034644632,0.0005654702,0.01593422,0.00014379753,0.0007808271,0.010515267],"study_design_scores_gemma":[0.000002211265,0.000037727747,0.99757034,0.0000032375133,0.000005866703,0.0004916078,0.000059300382,0.00055056025,0.0007568598,0.000036087757,0.00048358986,0.0000025931297],"about_ca_topic_score_codex":0.010345802,"about_ca_topic_score_gemma":0.024349764,"teacher_disagreement_score":0.010345802,"about_ca_system_score_codex":0.00028298082,"about_ca_system_score_gemma":0.000082160055,"threshold_uncertainty_score":0.020571172},"labels":[],"label_agreement":null},{"id":"W4394690309","doi":"10.3847/1538-4357/ad293a","title":"A Tale of Three Dwarfs: Cluster-based Star Formation Histories of Blue Compact Dwarf Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Ontario College of Art and Design","funders":"Smithsonian Astrophysical Observatory; Smithsonian Institution","keywords":"Astrophysics; Dwarf galaxy; Physics; Astronomy; Star formation; Cluster (spacecraft); Galaxy; Computer science","score_opus":0.010812728672747834,"score_gpt":0.22161039252949555,"score_spread":0.21079766385674772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394690309","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99941957,0.00003123826,0.00007837593,0.000008247279,4.2636032e-7,0.0000015282768,0.00009598306,0.000002925907,0.00036172607],"genre_scores_gemma":[0.99972445,0.000009895495,0.000049140974,0.0000034653472,7.711556e-7,8.793437e-7,0.00011436487,0.0000011682132,0.00009590078],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999039,0.000016756074,0.0000046452215,0.000033971897,0.000018187071,0.000022459579],"domain_scores_gemma":[0.9993892,0.00013870682,0.00016323081,0.000069809794,0.00008796007,0.00015116841],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028772783,0.000080197904,0.00013355914,0.0011584691,0.00032838667,0.0005174981,0.00022453813,0.00015228982,0.0008620581],"category_scores_gemma":[0.00094784616,0.00007065126,0.0001422131,0.0005434593,0.0003481529,0.00035790054,0.00043468561,0.00016966632,0.00012649303],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004984605,0.0000140340435,0.9942821,0.0000039746174,0.000016920201,0.00002659942,0.0004217119,0.00022045732,0.0019756446,0.000121630306,0.00006184952,0.0028051457],"study_design_scores_gemma":[5.494638e-7,0.000010031533,0.99920684,7.25064e-7,0.0000030436074,0.00002503989,0.00017250473,0.00023834866,0.00018971089,0.000042921605,0.00010867096,0.0000016801874],"about_ca_topic_score_codex":0.014155787,"about_ca_topic_score_gemma":0.02060934,"teacher_disagreement_score":0.014155787,"about_ca_system_score_codex":0.0005589001,"about_ca_system_score_gemma":0.00014804387,"threshold_uncertainty_score":0.028146744},"labels":[],"label_agreement":null},{"id":"W4394754835","doi":"10.3847/1538-4357/ad2859","title":"Data-driven Discovery of Diffuse Interstellar Bands with APOGEE Spectra","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Science Foundation","keywords":"Physics; Spectral line; Astrophysics; Interstellar medium; Astronomy; Interstellar cloud; Astrobiology; Galaxy","score_opus":0.014949920301125382,"score_gpt":0.23558313714954562,"score_spread":0.22063321684842024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394754835","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97485775,0.000093245115,0.019992696,0.00011424925,0.00001733451,0.000025169926,0.0024959326,0.0014521028,0.00095155695],"genre_scores_gemma":[0.981841,0.000024017736,0.011450183,0.000048943315,0.000007927486,0.000017226774,0.0060976124,0.00019499849,0.00031806607],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99900454,0.00016846297,0.0000514841,0.00041221414,0.00027155748,0.0000918425],"domain_scores_gemma":[0.9953935,0.0019042154,0.00065741653,0.0013259954,0.00045937896,0.00025959467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019061955,0.00046860497,0.00034893127,0.001122838,0.00035720042,0.0011417462,0.00091533375,0.0006493048,0.0010352249],"category_scores_gemma":[0.005200586,0.00035527517,0.00093856297,0.001016626,0.0004886923,0.0006768339,0.001179233,0.00071545335,0.00043293493],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004450202,0.00023619983,0.8674289,0.00011746734,0.00032788378,0.0007176559,0.00032925216,0.06920471,0.017874774,0.00266319,0.0039223954,0.0367326],"study_design_scores_gemma":[0.00007875287,0.0001209385,0.3870899,0.000028726015,0.00010707632,0.0006001047,0.00020295306,0.57725686,0.021505281,0.0036949962,0.009248007,0.00006638345],"about_ca_topic_score_codex":0.004020194,"about_ca_topic_score_gemma":0.004457099,"teacher_disagreement_score":0.004020194,"about_ca_system_score_codex":0.0006244188,"about_ca_system_score_gemma":0.00042164224,"threshold_uncertainty_score":0.010081053},"labels":[],"label_agreement":null},{"id":"W4394755235","doi":"10.3847/1538-4357/ad2bfd","title":"Model-independent Approach of the JUNO <sup>8</sup>B Solar Neutrino Program","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Russian Science Foundation; Lomonosov Moscow State University; Ministero degli Affari Esteri e della Cooperazione Internazionale; Ministry of Education, India; Joint Institute for Nuclear Research; Chulalongkorn University; Fonds De La Recherche Scientifique - FNRS; Chinese Academy of Sciences; Istituto Nazionale di Fisica Nucleare; Deutsche Forschungsgemeinschaft; National Natural Science Foundation of China; CAS Center for Excellence in Particle Physics; Wuyi University; Fonds Wetenschappelijk Onderzoek; Institut Català de Nanociència i Nanotecnologia; Suranaree University of Technology; Agencia Nacional de Investigación y Desarrollo; Univerzita Karlova v Praze; Shanghai Jiao Tong University; National Science Foundation","keywords":"Physics; Neutrino; Algorithm; Nuclear physics; Computer science","score_opus":0.022877231419354268,"score_gpt":0.2862828289000226,"score_spread":0.26340559748066833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394755235","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.49652088,0.00030301485,0.34518412,0.0012152215,0.00016350059,0.00026658492,0.0034185504,0.0017222303,0.15120599],"genre_scores_gemma":[0.89950943,0.00015011341,0.085718915,0.00015652526,0.000048546637,0.00019403956,0.0025519622,0.00032563982,0.011344803],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998566,0.00004498976,0.0000030735919,0.000021900094,0.00005179964,0.000021579735],"domain_scores_gemma":[0.9997551,0.00006601626,0.000031082098,0.000055580404,0.00006444864,0.000027711245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00053463347,0.00026036188,0.00025222352,0.00022997722,0.00037076513,0.0006801219,0.000878913,0.00028764937,0.003874158],"category_scores_gemma":[0.0006681345,0.00019131743,0.000599591,0.00025211726,0.00022287043,0.0004818853,0.00053580507,0.00044759587,0.00038910442],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005897808,0.00027839924,0.02511954,0.00020876896,0.00013084403,0.00030548807,0.0002468051,0.67678034,0.011759673,0.21969618,0.009974444,0.05490977],"study_design_scores_gemma":[0.000027178632,0.00004026487,0.0026617376,0.000007999866,0.00001834913,0.000022911663,0.000040729166,0.97277087,0.0016741205,0.0157335,0.0069903065,0.000012102926],"about_ca_topic_score_codex":0.008883472,"about_ca_topic_score_gemma":0.015669376,"teacher_disagreement_score":0.008883472,"about_ca_system_score_codex":0.0007354263,"about_ca_system_score_gemma":0.0012605926,"threshold_uncertainty_score":0.017663538},"labels":[],"label_agreement":null},{"id":"W4394761212","doi":"10.3847/1538-4357/ad28c2","title":"A Perspective on the Milky Way Bulge Bar as Seen from the Neutron-capture Elements Cerium and Neodymium with APOGEE","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Agencia Nacional de Investigación y Desarrollo; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Banco Santander; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ministerio de Ciencia e Innovación; Carnegie Institution of Washington; University of Utah; Centro de Astrofísica y Tecnologías Afines; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Agencia Estatal de Investigación; Yale University","keywords":"Bulge; Physics; Metallicity; Milky Way; Astrophysics; Stars; Population; Neodymium; Supernova","score_opus":0.007488197931395881,"score_gpt":0.21913646887488572,"score_spread":0.21164827094348984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394761212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.995551,0.0013843403,0.00043091178,0.00023039532,0.000009402921,0.0000014313484,0.00013722625,0.000009638426,0.0022457184],"genre_scores_gemma":[0.9984617,0.0005389474,0.00032425858,0.000060441645,0.000012696266,0.0000010310416,0.00016209813,0.000009242537,0.00042956075],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985874,0.00002584255,0.000004334204,0.000052487383,0.000022535372,0.000036070607],"domain_scores_gemma":[0.9997714,0.000044736247,0.00006938832,0.000016067539,0.00006056186,0.00003782094],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024071538,0.00019863805,0.0003369345,0.0017697983,0.00042815454,0.0015170397,0.00026703638,0.00030103078,0.0009003304],"category_scores_gemma":[0.000421279,0.000106829284,0.00024406913,0.0011807358,0.00078656897,0.00068074407,0.00094604574,0.00025617442,0.00017526212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029605988,0.000022264776,0.9215979,0.00010613798,0.00015173407,0.000856328,0.0035604602,0.0009611112,0.04569002,0.0027900129,0.0003969184,0.023571042],"study_design_scores_gemma":[0.0000024557476,0.000046542988,0.9904073,0.000025944557,0.00002545682,0.0003387636,0.00245764,0.0005179797,0.0014558096,0.00062313926,0.0040892344,0.000009775898],"about_ca_topic_score_codex":0.011308645,"about_ca_topic_score_gemma":0.01731281,"teacher_disagreement_score":0.011308645,"about_ca_system_score_codex":0.0007008534,"about_ca_system_score_gemma":0.00017246284,"threshold_uncertainty_score":0.022485614},"labels":[],"label_agreement":null},{"id":"W4394867868","doi":"10.3847/1538-4357/ad5c65","title":"Constraining Near-simultaneous Radio Emission from Short Gamma-Ray Bursts Using CHIME/FRB","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; York University; University of Toronto; Canadian Institute for Advanced Research; McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Canada Research Chairs; Smithsonian Astrophysical Observatory; McGill University; Canadian Institute for Advanced Research; Fonds de recherche du Québec – Nature et technologies; Alfred P. Sloan Foundation; University of Toronto; Research Corporation for Science Advancement; National Science Foundation","keywords":"Astrophysics; Physics; Gamma ray; Astronomy","score_opus":0.019784940592453427,"score_gpt":0.2651623527705763,"score_spread":0.2453774121781229,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394867868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9684931,0.00047897946,0.017088715,0.00015236415,0.000020415904,0.000052795785,0.006874999,0.0010184193,0.005820167],"genre_scores_gemma":[0.9708773,0.0001057195,0.016308377,0.00008296373,0.0000150534715,0.00003156651,0.011665518,0.00014511071,0.0007684164],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955267,0.000031746982,0.000009022313,0.0001349569,0.00015053576,0.00012100908],"domain_scores_gemma":[0.9991769,0.00013380399,0.00017905618,0.000137608,0.00012345165,0.00024917806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009567281,0.00063460274,0.0005875164,0.0019076321,0.0007758999,0.00091304426,0.0007450716,0.00045855742,0.0016505513],"category_scores_gemma":[0.0013748948,0.0005407716,0.000649152,0.0013264928,0.00036359995,0.0002624159,0.0010442093,0.00049221824,0.00054375903],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00073576433,0.00018714393,0.8010856,0.00014166163,0.00062895217,0.0005989582,0.00031011816,0.058708858,0.085989855,0.0021054957,0.004703737,0.04480385],"study_design_scores_gemma":[0.00008265969,0.00006790095,0.90357924,0.000041094478,0.00012196682,0.00023461881,0.00014276702,0.07643689,0.007702615,0.0006299372,0.010873092,0.00008726274],"about_ca_topic_score_codex":0.1926458,"about_ca_topic_score_gemma":0.32586813,"teacher_disagreement_score":0.1926458,"about_ca_system_score_codex":0.0013101958,"about_ca_system_score_gemma":0.0015751048,"threshold_uncertainty_score":0.38304895},"labels":[],"label_agreement":null},{"id":"W4394882155","doi":"10.3847/1538-4357/ad2fa1","title":"The Reservoir of the Per-emb-2 Streamer","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Geology; Materials science; Analytical Chemistry (journal); Chemistry; Chromatography","score_opus":0.009941311101171633,"score_gpt":0.2511009992954377,"score_spread":0.2411596881942661,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394882155","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98032093,0.00007601427,0.0019848545,0.00006586937,0.000016420843,0.000011533692,0.0016181072,0.0008595297,0.0150466375],"genre_scores_gemma":[0.98402655,0.000044666423,0.0039579663,0.000034176268,0.000014370705,0.000008252197,0.0027826093,0.00017201641,0.008959307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999516,0.0000031176132,0.0000015621097,0.000016574622,0.00001279414,0.000014446829],"domain_scores_gemma":[0.9998858,0.000011959185,0.00002397031,0.000019282737,0.000025787904,0.000033198172],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008999683,0.0001273715,0.00017653899,0.0002747576,0.00023221187,0.0004377438,0.00033539825,0.00016774566,0.005982258],"category_scores_gemma":[0.00017645939,0.00013231674,0.00009504731,0.00024425075,0.000082748964,0.00053843396,0.0003399709,0.0002086918,0.0012384151],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015863675,0.00028633134,0.5342097,0.00015121199,0.00007610773,0.0014941635,0.001074304,0.0049307,0.31045827,0.007156104,0.018733544,0.119843155],"study_design_scores_gemma":[0.000045307606,0.00014684146,0.8198237,0.0000323021,0.00004423354,0.00049746793,0.00028135622,0.030941185,0.09037255,0.0011221609,0.05666408,0.000028855156],"about_ca_topic_score_codex":0.0021996463,"about_ca_topic_score_gemma":0.0031398314,"teacher_disagreement_score":0.005982258,"about_ca_system_score_codex":0.00028311386,"about_ca_system_score_gemma":0.00012982864,"threshold_uncertainty_score":0.020012617},"labels":[],"label_agreement":null},{"id":"W4394882310","doi":"10.3847/1538-4357/ad2a7b","title":"EPOCHS. II. The Ultraviolet Luminosity Function from 7.5 &lt; z &lt; 13.5 Using 180 arcmin<sup>2</sup> of Deep, Blank Fields from the PEARLS Survey and Public JWST Data","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":115,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Chinese Academy of Sciences; National Aeronautics and Space Administration; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; National Natural Science Foundation of China; United States-Israel Binational Science Foundation; Goddard Space Flight Center; Smithsonian Institution; Chinese Academy of Sciences South America Center for Astronomy; European Research Council; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Reionization; Redshift; Galaxy; James Webb Space Telescope; Star formation; Luminosity function; Hubble Ultra-Deep Field; Cosmic variance; Astronomy; Luminosity; Galaxy formation and evolution; Spitzer Space Telescope; Advanced Camera for Surveys; Hubble Deep Field; Telescope","score_opus":0.025173610136919024,"score_gpt":0.23208834852292667,"score_spread":0.20691473838600766,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394882310","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96554726,0.0002146006,0.0017911759,0.00007980542,0.000017062483,0.000042502408,0.026307883,0.000559378,0.005440303],"genre_scores_gemma":[0.9142348,0.0001023533,0.0032045604,0.00006901854,0.00003068389,0.000040721872,0.079137206,0.0001297923,0.0030508728],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998294,0.000010582426,0.00001113469,0.000046168298,0.000051824718,0.000050856033],"domain_scores_gemma":[0.99936825,0.000061034705,0.00020845947,0.00008881565,0.00013923709,0.0001341236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031203488,0.00021529195,0.00021781008,0.0018915235,0.00025639115,0.00074297923,0.0002612389,0.00020022278,0.0040210267],"category_scores_gemma":[0.0005888768,0.00013441143,0.00046210512,0.0010203506,0.00020475958,0.00031017937,0.0004520258,0.00026795221,0.0015214743],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041027195,0.00008470761,0.941374,0.00007914924,0.000177402,0.00024919683,0.00024185001,0.00187898,0.011006458,0.00049221015,0.011272805,0.03273295],"study_design_scores_gemma":[0.000005825502,0.000014812547,0.9951379,0.0000041593817,0.000017444143,0.000065136934,0.000039406965,0.0009741744,0.0013733371,0.000048004647,0.0023168116,0.000002993],"about_ca_topic_score_codex":0.009093743,"about_ca_topic_score_gemma":0.019880926,"teacher_disagreement_score":0.009093743,"about_ca_system_score_codex":0.00028367018,"about_ca_system_score_gemma":0.00016833753,"threshold_uncertainty_score":0.018081605},"labels":[],"label_agreement":null},{"id":"W4394882602","doi":"10.3847/1538-4357/ad3440","title":"White Dwarf Merger Remnants: The DAQ Subclass","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Diverse Scientific and Economic Studies","field":"Economics, Econometrics and Finance","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Université de Montréal","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Subclass; White dwarf; White (mutation); Biology; Astrophysics; Physics; Genetics; Stars; Antibody","score_opus":0.02809667544238647,"score_gpt":0.21233256792154231,"score_spread":0.18423589247915584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394882602","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990114,0.00020022425,0.0001416273,0.000046980873,0.000004146678,0.0000055949495,0.0000755664,0.0000059694057,0.0005083486],"genre_scores_gemma":[0.9996879,0.000048126734,0.000042990046,0.000024394978,0.000008974069,0.000001217946,0.00009397782,0.0000024933354,0.00008998893],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970514,0.00003191539,0.00003453847,0.00008795943,0.0000587518,0.000081593615],"domain_scores_gemma":[0.9984876,0.00025721715,0.00058292015,0.00017135189,0.00017226207,0.00032873673],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006610082,0.00021245745,0.0003173847,0.0016113519,0.0007466698,0.000770088,0.0003017526,0.0002696678,0.0013220651],"category_scores_gemma":[0.0020462566,0.00013067419,0.00015960954,0.000865061,0.0009568886,0.00039040227,0.0011055487,0.00033583117,0.00030470797],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002241841,0.000034897774,0.9860533,0.000016594006,0.000032602093,0.0022390983,0.00069848157,0.000056257653,0.005006065,0.00062302616,0.00025611563,0.0047593936],"study_design_scores_gemma":[0.0000141559885,0.000105494,0.98611844,0.00001535042,0.000030081963,0.008054049,0.0011494254,0.00028477405,0.0014492781,0.00067623646,0.002092871,0.000009831354],"about_ca_topic_score_codex":0.0034533858,"about_ca_topic_score_gemma":0.0025384862,"teacher_disagreement_score":0.0034533858,"about_ca_system_score_codex":0.00034257516,"about_ca_system_score_gemma":0.00018827774,"threshold_uncertainty_score":0.0068665743},"labels":[],"label_agreement":null},{"id":"W4394893571","doi":"10.3847/1538-4357/ad2857","title":"The Initial Conditions of Clustered Core Collapse: Multiwavelength Analysis of Oph A SM1N and N6 at 100 au Resolution","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; University of Toronto","funders":"","keywords":"Astrophysics; Ophiuchus; Physics; Protostar; Submillimeter Array; Millimeter; Molecular cloud; Hydrostatic equilibrium; Star formation; Radiative transfer; Inner core; RADIUS; Mean kinetic temperature; Stars; Optics; Astronomy","score_opus":0.025241376913020742,"score_gpt":0.30547080851565056,"score_spread":0.2802294316026298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394893571","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99929047,0.00001533827,0.00021694314,0.000005757954,6.6224203e-7,0.0000028068557,0.000078073164,0.000015024697,0.00037475582],"genre_scores_gemma":[0.99934417,0.000007100978,0.0002928634,0.0000048510897,0.0000010902422,0.0000022791876,0.0002319621,0.0000047525996,0.00011105193],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999434,0.000003970293,0.0000023597172,0.000013876104,0.000018453904,0.000017961964],"domain_scores_gemma":[0.9998203,0.00002410458,0.00003707574,0.000016108555,0.0000293684,0.000073098745],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015119597,0.0002162987,0.00018361572,0.00041811995,0.00042208037,0.0003226284,0.00039584792,0.00021080223,0.0009470748],"category_scores_gemma":[0.00036005315,0.0002116019,0.00033468517,0.0002016111,0.00019611606,0.00018198637,0.0004113537,0.00022482799,0.00016048155],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039060635,0.00018182509,0.8143674,0.000049438782,0.00013051434,0.0012601746,0.00045416213,0.037245788,0.13697407,0.0008104141,0.00048829097,0.0076473],"study_design_scores_gemma":[0.00001276851,0.00004607511,0.91524416,0.0000046333384,0.000013246101,0.00017316049,0.00018528699,0.07908125,0.0047309548,0.00020484965,0.00029279848,0.00001077894],"about_ca_topic_score_codex":0.010228838,"about_ca_topic_score_gemma":0.011981589,"teacher_disagreement_score":0.010228838,"about_ca_system_score_codex":0.00059755176,"about_ca_system_score_gemma":0.00017500512,"threshold_uncertainty_score":0.020338595},"labels":[],"label_agreement":null},{"id":"W4394924638","doi":"10.3847/1538-4357/ad323d","title":"Winds and Disk Turbulence Exert Equal Torques on Thick Magnetically Arrested Disks","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":18,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Nuclear Safety and Security Commission; Northwestern University; Office of Science; National Aeronautics and Space Administration; Smithsonian Astrophysical Observatory; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Turbulence; Torque; Physics; Mechanics; Thermodynamics","score_opus":0.012336418090527164,"score_gpt":0.24941967752447064,"score_spread":0.23708325943394348,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394924638","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987859,0.00002582881,0.00022852667,0.00004309445,0.0000039818487,0.000004953591,0.00003775132,0.000018034267,0.0008520118],"genre_scores_gemma":[0.9996388,0.00001647771,0.00012668253,0.000013070604,0.0000029044443,0.0000036725703,0.00004858283,0.000009894195,0.00013986898],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998871,0.000020075584,0.0000073367387,0.000016334929,0.000018383325,0.000050769606],"domain_scores_gemma":[0.9995191,0.00014653872,0.000087937115,0.000039403334,0.00003953926,0.00016745339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018439806,0.00040635263,0.00046551734,0.00041817193,0.00064424844,0.0012427812,0.0004140739,0.0004570307,0.0013744491],"category_scores_gemma":[0.001359397,0.0003371284,0.00046432033,0.00020658491,0.0010276728,0.0006203342,0.00078421034,0.00057715253,0.0001455912],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012468876,0.00038806393,0.09137551,0.00009178003,0.0002676524,0.0014556831,0.00039065833,0.84158516,0.05401974,0.0041964375,0.00068671565,0.0042957077],"study_design_scores_gemma":[0.0002763404,0.00053397386,0.055334512,0.000023935361,0.00008911794,0.00010959467,0.00042594748,0.9351175,0.006163881,0.0014331753,0.0004407705,0.000051149975],"about_ca_topic_score_codex":0.007755243,"about_ca_topic_score_gemma":0.0042930422,"teacher_disagreement_score":0.007755243,"about_ca_system_score_codex":0.00065110996,"about_ca_system_score_gemma":0.00039072733,"threshold_uncertainty_score":0.015420198},"labels":[],"label_agreement":null},{"id":"W4394964720","doi":"10.3847/1538-4357/ad323e","title":"Erratum: “Inferences from Surface Brightness Fluctuations of Zwicky 3146 via the Sunyaev–Zel’dovich Effect and X-Ray Observations” (2023, ApJ, 951, 41)","year":2024,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Surface brightness; Astrophysics; Physics; Environmental science; Galaxy","score_opus":0.010668233051733355,"score_gpt":0.23430981615554344,"score_spread":0.22364158310381008,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4394964720","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0016226228,0.0023544268,0.0007238415,0.06428161,0.88668543,0.00005240396,0.005690195,0.00048763043,0.038101926],"genre_scores_gemma":[0.026480336,0.008965511,0.0049434993,0.073483855,0.1538349,0.00017962357,0.016296366,0.002025417,0.71379054],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9988475,0.000107744265,0.00021833231,0.00014704315,0.00059359404,0.00008573467],"domain_scores_gemma":[0.9927933,0.001379699,0.00050858763,0.0004589342,0.0044884244,0.00037111435],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014190625,0.0015469452,0.00073092774,0.0029829694,0.0034635784,0.002606447,0.0015115876,0.0021290195,0.045392968],"category_scores_gemma":[0.019311057,0.00055643084,0.000820688,0.0020874378,0.0009768956,0.00209706,0.0012121473,0.0042747282,0.034152057],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024246172,0.0000044614694,0.00016370794,0.00002692605,0.0000027890264,0.00011365551,0.00001907663,0.000022764554,0.000058699665,0.0005523287,0.99550676,0.003504621],"study_design_scores_gemma":[0.000018457467,0.000014816487,0.003189694,0.00015795679,0.000018637995,0.00020109062,0.00015157243,0.00013412088,0.00042428053,0.0011375297,0.9945201,0.000031661453],"about_ca_topic_score_codex":0.037562244,"about_ca_topic_score_gemma":0.043955814,"teacher_disagreement_score":0.045392968,"about_ca_system_score_codex":0.0024501837,"about_ca_system_score_gemma":0.0027454554,"threshold_uncertainty_score":0.15185457},"labels":[],"label_agreement":null},{"id":"W4395002295","doi":"10.3847/1538-4357/ad34d6","title":"Hα Time Delays of Active Galactic Nuclei from the Zwicky Transient Facility Broadband Photometry","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Leibniz-Gemeinschaft; Deutsches Elektronen-Synchrotron; Institut National de Physique Nucléaire et de Physique des Particules; University of Colorado Boulder; National Astronomical Observatories, Chinese Academy of Sciences; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; Leibniz-Institut für Astrophysik Potsdam; People's Government of Yunnan Province; New Mexico State University; Nanjing University; Smithsonian Astrophysical Observatory; National Development and Reform Commission; Yale University; University of Toronto; Stockholms Universitet; Chinese Academy of Sciences; Smithsonian Institution; National Natural Science Foundation of China; École Polytechnique Fédérale de Lausanne; Space Telescope Science Institute; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Harvard University; China National Textile and Apparel Council; National Science Foundation; Yunnan University; California Institute of Technology; Ohio State University; Trinity College Dublin","keywords":"Photometry (optics); Broadband; Physics; Transient (computer programming); Active galactic nucleus; Astrophysics; Astronomy; Galaxy; Computer science; Optics; Stars","score_opus":0.007199311722012104,"score_gpt":0.21244020771031202,"score_spread":0.20524089598829992,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395002295","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99298453,0.000078711695,0.003653672,0.000013247343,0.000005806613,0.000007716193,0.0019894491,0.00012857332,0.0011384161],"genre_scores_gemma":[0.99349964,0.000029755025,0.0019141064,0.0000047013514,0.000004109153,0.0000073729957,0.004077407,0.000020237518,0.00044265235],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999892,0.000007990278,0.000005370162,0.000036509475,0.000028795674,0.000029281737],"domain_scores_gemma":[0.9996296,0.00004867356,0.00014029533,0.000051530766,0.00007261127,0.000057344245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025513532,0.00018889396,0.000119844015,0.001232358,0.00014468237,0.00028186766,0.00023826257,0.000116926145,0.0013829304],"category_scores_gemma":[0.00086840376,0.00008187317,0.00015133979,0.0005938244,0.0000858372,0.00022735594,0.00024629975,0.00014121691,0.00033270544],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021240741,0.000024797573,0.93503726,0.000026835643,0.00008108248,0.0001490813,0.00013565646,0.004818539,0.021378886,0.00046963987,0.0012648017,0.03640099],"study_design_scores_gemma":[0.000003356201,0.000016745993,0.9881209,0.0000048156166,0.000011365365,0.000056743374,0.00004725752,0.006377147,0.0042632623,0.00009521106,0.0009979971,0.0000052675223],"about_ca_topic_score_codex":0.011948583,"about_ca_topic_score_gemma":0.01635561,"teacher_disagreement_score":0.011948583,"about_ca_system_score_codex":0.000429347,"about_ca_system_score_gemma":0.0001390293,"threshold_uncertainty_score":0.023758054},"labels":[],"label_agreement":null},{"id":"W4395021910","doi":"10.3847/1538-4357/ad4a77","title":"Multiphase Black Hole Feedback and a Bright [C ii] Halo in a LoBAL Quasar at z ∼ 6.6","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":22,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Università degli Studi di Trieste; Université de Montréal; Istituto Nazionale di Astrofisica","keywords":"Astrophysics; Physics; Quasar; Supermassive black hole; Halo; Galaxy; Accretion (finance); Outflow; Black hole (networking); Active galactic nucleus; Luminosity; Astronomy","score_opus":0.008958779947356985,"score_gpt":0.23055663745128838,"score_spread":0.2215978575039314,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395021910","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996618,0.000029195397,0.00005278372,0.0000280471,0.0000022651138,0.000002233568,0.000042817566,0.0000093171275,0.0001716051],"genre_scores_gemma":[0.9998628,0.0000094845045,0.000043519885,0.000011482381,0.0000046383107,5.64736e-7,0.000034861492,0.0000011227324,0.000031497737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994504,0.000004937335,0.0000024516585,0.000012228532,0.000010987363,0.000024296063],"domain_scores_gemma":[0.9996511,0.000033352866,0.000102396705,0.00001532073,0.00002488012,0.00017298448],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020362239,0.00023983775,0.00021967609,0.00087252253,0.00056662096,0.0005037983,0.00024080904,0.00031776042,0.00085702445],"category_scores_gemma":[0.00026422023,0.00017366151,0.00019902537,0.00026887527,0.00036883954,0.00017694428,0.00050160824,0.00032676893,0.00012207759],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020080856,0.00017671389,0.96758044,0.000011233437,0.000038583566,0.003818362,0.00032226264,0.00023949257,0.025029698,0.00013893879,0.00017650555,0.0022669707],"study_design_scores_gemma":[0.000003963101,0.00006187449,0.9982168,0.0000019996448,0.000006277923,0.0008096539,0.00009727542,0.00034915624,0.00031679904,0.000042599222,0.00009003681,0.0000035557816],"about_ca_topic_score_codex":0.0038158929,"about_ca_topic_score_gemma":0.0053133164,"teacher_disagreement_score":0.0038158929,"about_ca_system_score_codex":0.000230603,"about_ca_system_score_gemma":0.000082191626,"threshold_uncertainty_score":0.0075873733},"labels":[],"label_agreement":null},{"id":"W4395034777","doi":"10.3847/1538-4357/ad28b2","title":"High-cadence Timing of Binary Pulsars with CHIME","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"University of British Columbia; McGill University","funders":"Precursory Research for Embryonic Science and Technology; Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Alliance de recherche numérique du Canada; University of Toronto; Smithsonian Astrophysical Observatory; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Cadence; Binary number; Astrophysics; Astronomy; Geology; Physics; Mathematics; Arithmetic; Acoustics","score_opus":0.012674189721975218,"score_gpt":0.3081072462521385,"score_spread":0.2954330565301633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395034777","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9936838,0.00012269079,0.0010227056,0.00005742844,0.00001307438,0.000019308884,0.0008562241,0.00015043347,0.0040742657],"genre_scores_gemma":[0.9969613,0.000031939846,0.001194867,0.000022879034,0.000006176729,0.000008495344,0.0010656819,0.000022530494,0.00068612036],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997948,0.000011364037,0.0000034310353,0.000057613735,0.00009257158,0.00004016391],"domain_scores_gemma":[0.9996563,0.000038044553,0.000070752234,0.000059281574,0.00008983808,0.00008566967],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000290217,0.00017034651,0.00026919515,0.0008206267,0.0006393757,0.0004309394,0.0003337557,0.00021041468,0.0011391812],"category_scores_gemma":[0.0007278673,0.00023751568,0.00008216256,0.00062614406,0.00031036482,0.00017739482,0.00044604315,0.0003221827,0.00019726023],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007628936,0.00015410146,0.53543884,0.00008723313,0.00016608194,0.0006019531,0.00070997083,0.0024420803,0.4086986,0.0013639145,0.0032728077,0.046301574],"study_design_scores_gemma":[0.000023105944,0.00003855645,0.97995824,0.000003402937,0.000018192277,0.00015229592,0.000034209523,0.0026093528,0.012199015,0.0000991241,0.004847946,0.000016640824],"about_ca_topic_score_codex":0.06292925,"about_ca_topic_score_gemma":0.17150536,"teacher_disagreement_score":0.06292925,"about_ca_system_score_codex":0.0011975016,"about_ca_system_score_gemma":0.00055442523,"threshold_uncertainty_score":0.12512589},"labels":[],"label_agreement":null},{"id":"W4395034978","doi":"10.3847/1538-4357/ad35b8","title":"The Hobby–Eberly Telescope VIRUS Parallel Survey (HETVIPS)*","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Brookhaven National Laboratory; Department of Mechanical Engineering, University of Texas at Austin; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Gordon and Betty Moore Foundation; Queen's University Belfast; Durham University; York University; Space Telescope Science Institute; New Mexico State University; University of Portsmouth; Ohio State University; University of Texas at Austin; Los Alamos National Laboratory; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Mellon University; Harvard University; Queen's University; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; National Central University; Max-Planck-Institut für Astrophysik; Eötvös Loránd Tudományegyetem; National Science Foundation","keywords":"Hobby; Telescope; Astronomy; Physics; Astrophysics; Art; Visual arts","score_opus":0.01896318876291588,"score_gpt":0.29114079178691116,"score_spread":0.2721776030239953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395034978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.73524994,0.0008313483,0.015080726,0.00029229696,0.00018130067,0.0005537377,0.21367171,0.0017221518,0.032416776],"genre_scores_gemma":[0.560323,0.0006027467,0.039807487,0.00023025472,0.00020200538,0.0003821983,0.37965837,0.0007493903,0.018044533],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970055,0.000027802113,0.000011245491,0.00008276638,0.00012043414,0.00005728414],"domain_scores_gemma":[0.9993223,0.000052339237,0.00013720147,0.00013540674,0.00017584086,0.00017685124],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004735933,0.0003077061,0.00021411772,0.001433698,0.0005802706,0.00069339003,0.00040138135,0.00018196485,0.0053793737],"category_scores_gemma":[0.00066990854,0.0003145207,0.00027315025,0.001333645,0.00018489773,0.00045633546,0.0009409017,0.00037005643,0.0021802867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009215191,0.00027112875,0.5449056,0.00040871926,0.00032179838,0.0008442572,0.0010267864,0.0038064776,0.070412636,0.004590442,0.17225671,0.20023401],"study_design_scores_gemma":[0.0000712363,0.00010414701,0.8539412,0.000051948384,0.000036558587,0.00026729453,0.00021549755,0.0035489327,0.007889786,0.0006209073,0.1332275,0.000024983054],"about_ca_topic_score_codex":0.029681155,"about_ca_topic_score_gemma":0.04601147,"teacher_disagreement_score":0.029681155,"about_ca_system_score_codex":0.00051463937,"about_ca_system_score_gemma":0.0009464812,"threshold_uncertainty_score":0.059016764},"labels":[],"label_agreement":null},{"id":"W4395065138","doi":"10.3847/1538-4357/ad3d56","title":"An ALMA Search for Substructure and Fragmentation in Starless Cores in Orion B North","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"Canadian Space Agency; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Science Council; National Radio Astronomy Observatory; Canadian Foundation for AIDS Research; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Science Foundation","keywords":"Ophiuchus; Physics; Astrophysics; Substructure; Star formation; Molecular cloud; Population; Context (archaeology); Astronomy; Stars; Geology","score_opus":0.016044653248975825,"score_gpt":0.293620254503108,"score_spread":0.2775756012541322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395065138","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996222,0.000016513413,0.00012931469,0.000011512125,5.778856e-7,0.000002098306,0.000042043393,0.000008356166,0.00016728598],"genre_scores_gemma":[0.99957544,0.0000064065334,0.0002575529,0.0000051559155,0.0000013877317,0.0000012847204,0.00008960698,0.0000018050064,0.00006132388],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999268,0.0000136005365,0.000003158583,0.000026471878,0.00001702293,0.000012916147],"domain_scores_gemma":[0.9995982,0.000072118055,0.00013619706,0.000038063463,0.000031667234,0.00012373996],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024287391,0.00014321643,0.00014074465,0.0006663377,0.00039001153,0.00040272434,0.00028617145,0.00021126283,0.0007386407],"category_scores_gemma":[0.0005632336,0.00011996271,0.00018389674,0.000291053,0.00019355613,0.00019445662,0.00033829777,0.000117401745,0.00008683295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011810956,0.000054812077,0.9811632,0.000007663845,0.000034136505,0.00014792375,0.00017121287,0.0016154213,0.012618187,0.00021465588,0.00012002032,0.003734661],"study_design_scores_gemma":[0.000016159644,0.000059789858,0.9870797,0.000003812074,0.000014245937,0.00007335785,0.00012470038,0.010428164,0.0015929578,0.00021244762,0.00039011988,0.0000045954685],"about_ca_topic_score_codex":0.009002165,"about_ca_topic_score_gemma":0.012347806,"teacher_disagreement_score":0.009002165,"about_ca_system_score_codex":0.00041636903,"about_ca_system_score_gemma":0.00018414557,"threshold_uncertainty_score":0.017899573},"labels":[],"label_agreement":null},{"id":"W4395081625","doi":"10.3847/1538-4357/ad2e01","title":"Emulating Power Spectra for Prereconstructed and Postreconstructed Galaxy Samples","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Science and Technology Facilities Council; Youth Innovation Promotion Association of the Chinese Academy of Sciences; National Key Research and Development Program of China; China Scholarship Council; National Natural Science Foundation of China; Youth Innovation Promotion Association; Japan Society for the Promotion of Science; Ministry of Education, Culture, Sports, Science and Technology; University of Portsmouth","keywords":"Galaxy; Astrophysics; Spectral line; Power (physics); Environmental science; Astronomy; Physics","score_opus":0.008798298055467503,"score_gpt":0.2218284549210991,"score_spread":0.2130301568656316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395081625","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.53666294,0.00007680305,0.45510548,0.0001776342,0.000049664923,0.00006213268,0.00059404835,0.0039478275,0.0033234926],"genre_scores_gemma":[0.9032208,0.000048310332,0.09297725,0.000093748175,0.000015932257,0.00006179787,0.0010804235,0.001136768,0.0013649759],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996793,0.00007695744,0.000017142893,0.00006394823,0.00011642533,0.000046139186],"domain_scores_gemma":[0.9986796,0.00051512977,0.00015769164,0.000320394,0.00024369502,0.00008340491],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012770813,0.0006262413,0.00026595045,0.000631594,0.0002587896,0.00062722183,0.0011169704,0.0006429756,0.0029917522],"category_scores_gemma":[0.0052248426,0.00037125428,0.0006335178,0.00046310344,0.00055328174,0.001017486,0.0007606431,0.00057734037,0.00083098444],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065870694,0.0001478025,0.018547246,0.00011473714,0.00014223247,0.0007764952,0.00042594344,0.84820336,0.06472985,0.012377976,0.0013979699,0.05247764],"study_design_scores_gemma":[0.000021566522,0.000036172038,0.003940661,0.0000070501756,0.000011838155,0.000086194384,0.000024425,0.9587916,0.034494355,0.00180986,0.0007546342,0.00002159853],"about_ca_topic_score_codex":0.0018641842,"about_ca_topic_score_gemma":0.0012947601,"teacher_disagreement_score":0.0029917522,"about_ca_system_score_codex":0.00058376347,"about_ca_system_score_gemma":0.0004392465,"threshold_uncertainty_score":0.010008454},"labels":[],"label_agreement":null},{"id":"W4395455905","doi":"10.3847/1538-4357/ad2e94","title":"Small and Large Dust Cavities in Disks around Mid-M Stars in Taurus","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Key Research and Development Program of China; National Institutes of Natural Sciences; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; National Astronomical Observatory of Japan; European Commission; National Natural Science Foundation of China; National Radio Astronomy Observatory; Government of the United Kingdom; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; UK Research and Innovation; HORIZON EUROPE Framework Programme; Space Telescope Science Institute; National Science Foundation","keywords":"Stars; Astrophysics; Astronomy; Astrobiology; Physics","score_opus":0.016027483156547766,"score_gpt":0.2468727479577382,"score_spread":0.23084526480119044,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395455905","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996464,0.00008340735,0.00007153073,0.0000061648557,0.0000010743574,0.0000014260738,0.000054421293,0.000010228033,0.00012538744],"genre_scores_gemma":[0.9997373,0.000012747242,0.00014114482,0.0000036220908,0.0000033302679,0.0000015644611,0.000070186434,0.0000017757719,0.000028362645],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990606,0.0000093018325,0.0000074089276,0.000039248134,0.000016389668,0.000021711789],"domain_scores_gemma":[0.99961686,0.00007305196,0.0001444605,0.00003299172,0.00003510584,0.00009749633],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012217936,0.00022795526,0.00024778154,0.0011488402,0.000497561,0.00048420133,0.0003456265,0.0004266131,0.0006045731],"category_scores_gemma":[0.0004009687,0.00025235294,0.00022661818,0.0004043431,0.00030436885,0.00030184034,0.0005061687,0.00014702702,0.000152403],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040099514,0.00007298536,0.8819531,0.000042496205,0.000055823624,0.00068057346,0.00085126096,0.00042793417,0.108347334,0.000097789154,0.00015793653,0.00691173],"study_design_scores_gemma":[0.000008360133,0.00003800753,0.99761057,0.0000030942347,0.000010633933,0.00026279723,0.00016327927,0.0004762039,0.0012307285,0.000032446653,0.00016065422,0.0000031937384],"about_ca_topic_score_codex":0.0014117338,"about_ca_topic_score_gemma":0.0020678667,"teacher_disagreement_score":0.0014117338,"about_ca_system_score_codex":0.00022508646,"about_ca_system_score_gemma":0.00005699323,"threshold_uncertainty_score":0.0028070211},"labels":[],"label_agreement":null},{"id":"W4395463082","doi":"10.3847/1538-4357/ad3209","title":"Probing the Stellar Populations and Star Formation History of Early-type Galaxies at 0 &lt; z &lt; 1.1 in the Rest-frame Ultraviolet","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Astronomical Observatories, Chinese Academy of Sciences; Japan Society for the Promotion of Science; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; Japan Science and Technology Agency; Cabinet Office, Government of Japan; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; Academia Sinica; Princeton University; Canadian Foundation for AIDS Research; Ministry of Education, Culture, Sports, Science and Technology; Science and Technology Facilities Council; National Research Foundation; Toray Science Foundation; Compute Canada; National Research Foundation of Korea","keywords":"Rest frame; Rest (music); Astrophysics; Physics; Galaxy; Ultraviolet; Star (game theory); Star formation; Astronomy; Optics; Redshift","score_opus":0.016112885280917692,"score_gpt":0.22309315619181483,"score_spread":0.20698027091089713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395463082","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99939334,0.000012853142,0.000043900494,0.000008333173,4.0876736e-7,0.0000013509336,0.00034386246,0.000008644412,0.00018725546],"genre_scores_gemma":[0.9991715,0.00000867464,0.00008247429,0.0000055004703,0.0000013396719,0.0000018318025,0.00058049004,0.000002219993,0.00014607621],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999068,0.0000101692485,0.0000033134736,0.000025245192,0.000021330494,0.00003309414],"domain_scores_gemma":[0.9989134,0.000110681125,0.00038632355,0.000060989012,0.000120714605,0.0004078997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003346188,0.00016408591,0.00016445511,0.0008851704,0.00023844166,0.0004447921,0.00025672626,0.00024449165,0.0011102554],"category_scores_gemma":[0.0007202218,0.00011792257,0.00017747062,0.0005042816,0.000193553,0.00029227455,0.00034472055,0.000220095,0.000348166],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000067303634,0.000023721275,0.9943534,0.0000043057958,0.000014769933,0.000022445214,0.00012017707,0.00025423584,0.0035817053,0.00004960965,0.0001385042,0.0013698128],"study_design_scores_gemma":[5.5894395e-7,0.000007713996,0.99963784,3.9995703e-7,0.0000016802629,0.0000070707115,0.000018056522,0.00014946239,0.00013308643,0.0000053294048,0.000038044574,6.6137324e-7],"about_ca_topic_score_codex":0.010587313,"about_ca_topic_score_gemma":0.017930329,"teacher_disagreement_score":0.010587313,"about_ca_system_score_codex":0.00040183598,"about_ca_system_score_gemma":0.00011360144,"threshold_uncertainty_score":0.021051347},"labels":[],"label_agreement":null},{"id":"W4395480590","doi":"10.3847/1538-4357/ad3063","title":"Comprehensive High-resolution Chemical Spectroscopy of Barnard’s Star with SPIRou","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Institut national des sciences de l'Univers; Horizon 2020 Framework Programme; Fundação de Amparo à Pesquisa do Estado de Minas Gerais; Centre National de la Recherche Scientifique; Conselho Nacional de Desenvolvimento Científico e Tecnológico; National Aeronautics and Space Administration; Agence Nationale de la Recherche; Vanderbilt University","keywords":"Physics; Metallicity; Astrophysics; Stars; Exoplanet; Spectroscopy; Galaxy; Spectral resolution; Spectral line; Effective temperature; Astronomy","score_opus":0.008716033141443362,"score_gpt":0.22373739280004412,"score_spread":0.21502135965860075,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395480590","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982412,0.00004957407,0.00030691092,0.000019642588,0.0000038991134,0.0000041736175,0.0002417556,0.000032905653,0.0010998768],"genre_scores_gemma":[0.99822,0.00001586121,0.00088653516,0.000027059474,0.0000031537752,0.0000017591477,0.00044799442,0.000007614742,0.00039000198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999255,0.0000038472854,0.0000019094384,0.00002804492,0.000029177794,0.000011517672],"domain_scores_gemma":[0.99990237,0.0000050469985,0.000018971072,0.000007842871,0.000034765595,0.00003100484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009842764,0.00014913881,0.0002133124,0.0004894205,0.0005702219,0.00024835108,0.00018195237,0.00024694877,0.0005113047],"category_scores_gemma":[0.00008796447,0.00009746981,0.00012571648,0.00027087683,0.000108319844,0.00010620461,0.00027405095,0.00017707814,0.0003237805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002741891,0.00018070434,0.7120352,0.000039817067,0.00006818107,0.00088011374,0.00053769915,0.00075608207,0.25726357,0.00025417816,0.001117215,0.026593108],"study_design_scores_gemma":[0.000008302716,0.00013929274,0.9751012,0.0000067896763,0.000023198878,0.0008954009,0.00032051062,0.0029731372,0.017072022,0.0000858201,0.0033636077,0.000010888225],"about_ca_topic_score_codex":0.008914649,"about_ca_topic_score_gemma":0.018983474,"teacher_disagreement_score":0.008914649,"about_ca_system_score_codex":0.0002537847,"about_ca_system_score_gemma":0.000096011,"threshold_uncertainty_score":0.017725527},"labels":[],"label_agreement":null},{"id":"W4395668373","doi":"10.3847/1538-4357/ad2858","title":"The NANOGrav 12.5-Year Data Set: Dispersion Measure Misestimations with Varying Bandwidths","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"CCD and CMOS Imaging Sensors","field":"Engineering","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Science and Technology Facilities Council","keywords":"Measure (data warehouse); Dispersion (optics); Data set; Set (abstract data type); Physics; Statistics; Mathematics; Computer science; Optics; Data mining","score_opus":0.017080435134662095,"score_gpt":0.23052892263001662,"score_spread":0.21344848749535453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395668373","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99205846,0.00010442928,0.0038314941,0.000062122876,0.000025300003,0.00001035242,0.0026966953,0.00027799647,0.00093303435],"genre_scores_gemma":[0.9868057,0.000027732673,0.0036298288,0.000035601406,0.000012328957,0.00001980916,0.009092816,0.00008720844,0.0002889904],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9991092,0.00012227501,0.000087406515,0.0003019987,0.0003038163,0.000075276155],"domain_scores_gemma":[0.996915,0.0010468147,0.00060533243,0.0008162575,0.0004945628,0.00012193157],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015033645,0.00033962444,0.00041974394,0.0014541737,0.00040900445,0.00061108865,0.0005267057,0.0004642124,0.0005500755],"category_scores_gemma":[0.004734151,0.0001962833,0.00042490728,0.0014358425,0.00023673725,0.00044225663,0.0005045396,0.00045219687,0.00025668662],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084802957,0.00023100415,0.8342133,0.0001215776,0.00043817365,0.00050400035,0.00029514253,0.07862931,0.028708434,0.0012503172,0.005837097,0.04892366],"study_design_scores_gemma":[0.00004566986,0.000115834315,0.8700456,0.000027775559,0.00007703295,0.00041482417,0.0001257438,0.111723535,0.011695567,0.0005101157,0.0051581855,0.000060182083],"about_ca_topic_score_codex":0.00798362,"about_ca_topic_score_gemma":0.011380953,"teacher_disagreement_score":0.00798362,"about_ca_system_score_codex":0.000468556,"about_ca_system_score_gemma":0.00026376892,"threshold_uncertainty_score":0.015874326},"labels":[],"label_agreement":null},{"id":"W4395674252","doi":"10.3847/1538-4357/ad35bc","title":"A Steep Decline in the Galaxy Space Density beyond Redshift 9 in the CANUCS UV Luminosity Function","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":53,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Javna Agencija za Raziskovalno Dejavnost RS; Canadian Space Agency; Space Telescope Science Institute; Canarie; Canadian Foundation for AIDS Research; Japan Society for the Promotion of Science; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Redshift; Galaxy; Astronomy; James Webb Space Telescope; Luminosity function; Hubble Ultra-Deep Field; Cosmic variance; Galaxy formation and evolution; Hubble Deep Field","score_opus":0.008100750672019106,"score_gpt":0.21916765381022427,"score_spread":0.21106690313820517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395674252","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99704283,0.00010153258,0.00008282826,0.00003399602,0.0000034385291,0.0000031420873,0.000716566,0.00004504016,0.0019705396],"genre_scores_gemma":[0.9984034,0.000029079582,0.00010581596,0.000018327322,0.000003444512,0.000002670813,0.0011285448,0.00000748621,0.00030125998],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996854,0.000030917574,0.000009990651,0.00008219454,0.000097620534,0.000093936185],"domain_scores_gemma":[0.99858946,0.0001549013,0.00033665253,0.00020782954,0.00035737912,0.00035372723],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003219162,0.00022143562,0.00026513496,0.002679293,0.00043933673,0.0008593766,0.00042683198,0.0003496132,0.0022264344],"category_scores_gemma":[0.001482251,0.00012281281,0.00017991166,0.0013335941,0.00048672306,0.0003639688,0.000688551,0.0002485043,0.00044233634],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000086432665,0.000019388472,0.9811205,0.000014890033,0.000022753708,0.000061082384,0.000420874,0.00016896651,0.0050526126,0.00029609783,0.0010947996,0.011641486],"study_design_scores_gemma":[6.914345e-7,0.000008231109,0.9991835,0.0000032066296,0.000002268145,0.000022595319,0.000056194684,0.00012046762,0.00016716679,0.000020787116,0.00041325434,0.0000016715227],"about_ca_topic_score_codex":0.039330438,"about_ca_topic_score_gemma":0.052214492,"teacher_disagreement_score":0.039330438,"about_ca_system_score_codex":0.000659476,"about_ca_system_score_gemma":0.00031672817,"threshold_uncertainty_score":0.07820296},"labels":[],"label_agreement":null},{"id":"W4395675427","doi":"10.3847/1538-4357/ad3076","title":"Gas and Star Formation in Satellites of Milky Way Analogs","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Queen's University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; Royal Military College of Canada; University of Toronto","funders":"Agencia Estatal de Investigación; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministerio de Ciencia e Innovación; Royal Society; European Research Council; National Science Foundation","keywords":"Milky Way; Star (game theory); Astronomy; Physics; Astrophysics; Astrobiology; Galaxy","score_opus":0.010189475555932092,"score_gpt":0.2238666407033392,"score_spread":0.21367716514740712,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395675427","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99953187,0.0000316825,0.00009492173,0.00000572258,3.5746177e-7,9.0551447e-7,0.0000403761,0.000011888532,0.00028237497],"genre_scores_gemma":[0.9996575,0.000010646995,0.00014492092,0.0000025587904,6.2147126e-7,6.743865e-7,0.00009878168,0.000003991009,0.000080280304],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999535,0.000007318365,0.000002599037,0.000015897698,0.000011517335,0.000009120917],"domain_scores_gemma":[0.99978906,0.000038139413,0.0000837404,0.000025922398,0.000022336108,0.000040807645],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011052462,0.000106660314,0.00014278486,0.00047533272,0.00017788282,0.000514646,0.00021483959,0.0001730943,0.0010431032],"category_scores_gemma":[0.0005216912,0.00016941027,0.00013465826,0.00045635962,0.00026668757,0.00040184,0.00050915603,0.00012879951,0.00014321016],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000221423,0.00002872317,0.95739263,0.000027072105,0.00009080789,0.00024252344,0.0006051576,0.012139096,0.021826888,0.0005560891,0.00023937973,0.006630393],"study_design_scores_gemma":[0.000023059994,0.00007442672,0.9742727,0.000011003002,0.000029660801,0.00023362758,0.0004802904,0.018131642,0.004853822,0.00026771615,0.0016092133,0.000012757609],"about_ca_topic_score_codex":0.0058212844,"about_ca_topic_score_gemma":0.0062210388,"teacher_disagreement_score":0.0058212844,"about_ca_system_score_codex":0.0003783741,"about_ca_system_score_gemma":0.000100759535,"threshold_uncertainty_score":0.011574805},"labels":[],"label_agreement":null},{"id":"W4395685035","doi":"10.3847/1538-4357/ad3109","title":"Turbulence, and Proton and Electron Heating Rates in the Solar Corona: Analytical Approach","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Heliophysics Division; Arkansas NSF EPSCoR","keywords":"Corona (planetary geology); Proton; Electron; Turbulence; Physics; Nanoflares; Solar wind; Atmospheric sciences; Astrophysics; Computational physics; Environmental science; Plasma; Atomic physics; Coronal mass ejection; Meteorology; Nuclear physics; Astrobiology","score_opus":0.007947130880787266,"score_gpt":0.2567324595236761,"score_spread":0.24878532864288885,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395685035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4842826,0.0063369237,0.45266336,0.001773818,0.00022384616,0.00013534029,0.0002707067,0.0007227579,0.05359065],"genre_scores_gemma":[0.9635389,0.002495265,0.025297508,0.00015034445,0.00010121729,0.00007629862,0.000081606726,0.00007547598,0.008183387],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999331,0.00001550715,0.000005388888,0.000009404333,0.000019396382,0.000017150547],"domain_scores_gemma":[0.9997819,0.000088403336,0.00004647577,0.000018071409,0.00005438887,0.000010775299],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027654495,0.00066804525,0.00028008543,0.00063578296,0.00032432112,0.0007391692,0.00061063044,0.00063789,0.0013885457],"category_scores_gemma":[0.0014494329,0.00030720778,0.0005795971,0.00040576057,0.00054259726,0.00085755455,0.0005642661,0.0005621631,0.00027524892],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000050962994,0.00010762168,0.0053258208,0.00019246462,0.000052464875,0.0006173284,0.00033051622,0.82962084,0.022169499,0.117146894,0.0020496382,0.022335937],"study_design_scores_gemma":[0.000008028602,0.000011527496,0.0010427079,0.000017138465,0.000004962001,0.00004954452,0.000048756036,0.9882704,0.0010545637,0.008710806,0.00076976727,0.0000118498065],"about_ca_topic_score_codex":0.0053382507,"about_ca_topic_score_gemma":0.0026938731,"teacher_disagreement_score":0.0053382507,"about_ca_system_score_codex":0.00069031416,"about_ca_system_score_gemma":0.00085167476,"threshold_uncertainty_score":0.010614336},"labels":[],"label_agreement":null},{"id":"W4395959499","doi":"10.3847/1538-4357/ad3106","title":"ALMA Spectral Survey of an Eruptive Young Star, V883 Ori (ASSAY). I. What Triggered the Current Episode of Eruption?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Research Foundation of Korea","keywords":"Current (fluid); Astronomy; Astrophysics; Physics; Geology","score_opus":0.02217463558904595,"score_gpt":0.294735340927239,"score_spread":0.2725607053381931,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4395959499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99836165,0.00009443952,0.000073015355,0.00002148618,0.0000017344595,0.0000054982975,0.0008757583,0.000016966147,0.0005493421],"genre_scores_gemma":[0.99703395,0.00008412954,0.00043251406,0.000032137363,0.0000084493095,0.000006879729,0.0019014301,0.000007103858,0.0004934077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993277,0.0000051755615,0.000005029029,0.000019309187,0.00001997772,0.000017689625],"domain_scores_gemma":[0.99972063,0.000014967267,0.000118589036,0.00001946671,0.000050936895,0.000075476026],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013919274,0.000121347446,0.0001630643,0.0006426405,0.00030404894,0.0002502891,0.0001504044,0.0002254645,0.00045823428],"category_scores_gemma":[0.00017382287,0.0000830725,0.00013047847,0.0005110935,0.000088834924,0.00012535449,0.00021887703,0.00012424396,0.0003280825],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010794107,0.000052488664,0.9440198,0.00003182396,0.000021537628,0.0003678671,0.0004480609,0.000063343185,0.04405923,0.00004397591,0.00062668155,0.010157258],"study_design_scores_gemma":[0.0000012295585,0.000022700535,0.99858665,0.0000014627223,0.0000054389498,0.00014424544,0.00005770981,0.000068534646,0.0004515486,0.0000049453342,0.0006547713,7.8302764e-7],"about_ca_topic_score_codex":0.006626276,"about_ca_topic_score_gemma":0.015863568,"teacher_disagreement_score":0.006626276,"about_ca_system_score_codex":0.0002062944,"about_ca_system_score_gemma":0.00010874842,"threshold_uncertainty_score":0.013175428},"labels":[],"label_agreement":null},{"id":"W4396222274","doi":"10.3847/1538-4357/ad2b68","title":"An Angular Diameter Measurement of β UMa via Stellar Intensity Interferometry with the VERITAS Observatory","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Embry-Riddle Aeronautical University; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Observatory; Physics; Interferometry; Astronomy; Angular diameter; Angular resolution (graph drawing); Optics; Intensity interferometer; Intensity (physics); Astrophysics; Stars; Astronomical interferometer; Mathematics","score_opus":0.01940648618561163,"score_gpt":0.22229719000156212,"score_spread":0.20289070381595048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396222274","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9836367,0.00009891943,0.0065024327,0.00003095923,0.000013696945,0.000022483422,0.0017576747,0.00044981428,0.0074874023],"genre_scores_gemma":[0.98995346,0.000045578796,0.0076488797,0.000030698924,0.000015060969,0.000014085048,0.0017065533,0.000054442884,0.000531217],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971884,0.000018195327,0.0000115142375,0.00011791748,0.00010039607,0.00003310389],"domain_scores_gemma":[0.99946815,0.000046079273,0.00018190897,0.00008983351,0.00013364312,0.00008036574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040398267,0.00024066695,0.00020947766,0.0008957163,0.00036314165,0.0005032202,0.00050418044,0.00019148132,0.0014611051],"category_scores_gemma":[0.00052443286,0.0002807284,0.0002990476,0.00043323854,0.00024244009,0.00042432806,0.0006317728,0.00036143977,0.0004202576],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003076697,0.00005492298,0.6836111,0.00004928328,0.00012838333,0.0000942005,0.00027239937,0.002160788,0.28301436,0.00075082877,0.0009277455,0.028628413],"study_design_scores_gemma":[0.000039366947,0.00017457362,0.93445927,0.000016182932,0.0000824555,0.00021371283,0.00011221896,0.012698442,0.04836295,0.0001575435,0.0036594379,0.00002390515],"about_ca_topic_score_codex":0.0066980547,"about_ca_topic_score_gemma":0.013369355,"teacher_disagreement_score":0.0066980547,"about_ca_system_score_codex":0.00052424293,"about_ca_system_score_gemma":0.0002960463,"threshold_uncertainty_score":0.013318121},"labels":[],"label_agreement":null},{"id":"W4396230265","doi":"10.3847/1538-4357/ad36be","title":"Comparing Recent Pulsar Timing Array Results on the Nanohertz Stochastic Gravitational-wave Background","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":104,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"Division of Astronomical Sciences; Division of Mathematical Sciences; Office of Naval Research; Institut National de Physique Nucléaire et de Physique des Particules; Horizon 2020 Framework Programme; Goddard Space Flight Center; Jet Propulsion Laboratory; Directorate for Mathematical and Physical Sciences; Hellenic Foundation for Research and Innovation; Commonwealth Scientific and Industrial Research Organisation; Eötvös Loránd Tudományegyetem; Council for Higher Education; Istituto Nazionale di Astrofisica; Stavros Niarchos Foundation; College of Science, Oregon State University; Centre National d’Etudes Spatiales; University of Toronto; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Deutsche Forschungsgemeinschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Department of Atomic Energy, Government of India; European Research Council; Max-Planck-Gesellschaft; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; Department of Science and Technology, Ministry of Science and Technology, India; ASTRON; National Research Foundation; Agence Nationale de la Recherche; Gordon and Betty Moore Foundation; Ministero dell’Istruzione, dell’Università e della Ricerca; Australian Government; National Natural Science Foundation of China; John Templeton Foundation; European Commission; National Radio Astronomy Observatory; Associated Universities; Space Telescope Science Institute; Japan Society for the Promotion of Science; Oregon State University; Canadian Institute for Advanced Research; Texas Tech University; U.S. Naval Research Laboratory; Research Corporation for Science Advancement; National Aeronautics and Space Administration; Institute of Mathematical Sciences; Vanderbilt University; Alexander von Humboldt-Stiftung; Israel Academy of Sciences and Humanities; Alfred P. Sloan Foundation; Brinson Foundation; Swinburne University of Technology; University of Central Florida; Regione Autonoma della Sardegna; Simons Foundation; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Flatiron Health; California Institute of Technology; Royal Society; National Science Foundation","keywords":"Pulsar; Physics; Gravitational wave; Astrophysics; Noise (video); Gravitational wave background; Amplitude; Astronomy; Optics; Artificial intelligence; Computer science","score_opus":0.06787844182842213,"score_gpt":0.3424665068905915,"score_spread":0.2745880650621694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396230265","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8944429,0.001666795,0.055648543,0.0014242815,0.00042077678,0.00006198614,0.02112616,0.0012575955,0.023950996],"genre_scores_gemma":[0.9625924,0.0003900771,0.009722607,0.00040015325,0.00029464785,0.000068262176,0.024551522,0.00056628423,0.0014140205],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99770325,0.00045136557,0.00018794717,0.0006940523,0.00082603743,0.0001373718],"domain_scores_gemma":[0.9868024,0.0047418913,0.002828506,0.002476517,0.0025187547,0.0006319341],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0063213427,0.000451594,0.0005297945,0.0020830263,0.0004083809,0.0020498626,0.0009095598,0.0005685737,0.0015213072],"category_scores_gemma":[0.01398028,0.0003942425,0.0008953298,0.0033279732,0.00044062836,0.001364321,0.0018623157,0.0008180045,0.00073231914],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009282554,0.000102907616,0.8383519,0.00050247886,0.002168479,0.0005161902,0.0010820976,0.05551696,0.013443589,0.012277477,0.0098348735,0.065274775],"study_design_scores_gemma":[0.00006031999,0.00016308656,0.9151383,0.00011418288,0.0005902305,0.00038632474,0.0002414768,0.036070947,0.0066924244,0.003549784,0.036868267,0.00012466963],"about_ca_topic_score_codex":0.0051835277,"about_ca_topic_score_gemma":0.0072328355,"teacher_disagreement_score":0.0063213427,"about_ca_system_score_codex":0.00068712654,"about_ca_system_score_gemma":0.00043263414,"threshold_uncertainty_score":0.033430874},"labels":[],"label_agreement":null},{"id":"W4396511616","doi":"10.3847/1538-4357/ad2610","title":"The Atacama Cosmology Telescope: Mitigating the Impact of Extragalactic Foregrounds for the DR6 Cosmic Microwave Background Lensing Analysis","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":56,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"High Energy Physics; Office of Science; National Institute of Standards and Technology; Agencia Nacional de Investigación y Desarrollo; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; University of Toronto; National Research Foundation; U.S. Department of Energy; European Commission; National Energy Research Scientific Computing Center; National Science Foundation; Compute Canada; Japan Society for the Promotion of Science; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; University of Pennsylvania; Ministry of Education, Culture, Sports, Science and Technology; Princeton University; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Alfred P. Sloan Foundation; Government of Ontario","keywords":"Cosmic microwave background; Physics; Cosmology; Astronomy; Telescope; Astrophysics; COSMIC cancer database; Optics","score_opus":0.014908785779079253,"score_gpt":0.2712706728806569,"score_spread":0.2563618871015777,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396511616","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9729145,0.00013580012,0.019493693,0.00033551062,0.000032643322,0.000033699038,0.0017759888,0.0010190577,0.0042590983],"genre_scores_gemma":[0.96405625,0.00003684725,0.032350667,0.00006471193,0.000024974359,0.000019050001,0.0026219836,0.0001896487,0.00063584093],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99914503,0.0003868995,0.00003305855,0.00013612377,0.0002265457,0.000072305884],"domain_scores_gemma":[0.9969338,0.0013746266,0.00035765563,0.00064749795,0.00049513986,0.00019137027],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0028148768,0.00042720485,0.00035576915,0.0005183373,0.0003679261,0.0005815762,0.0009057973,0.00035070497,0.0017610404],"category_scores_gemma":[0.0055136704,0.0002528693,0.0006930537,0.0007110473,0.0003068018,0.0005945196,0.0006794073,0.0005671616,0.00033868322],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0020244217,0.0003103823,0.3734785,0.00029803265,0.0010748951,0.00061364425,0.00039496753,0.4959326,0.03661752,0.005359656,0.00686942,0.077025965],"study_design_scores_gemma":[0.00028647235,0.0005145352,0.2521682,0.000027664635,0.00020287369,0.00027503652,0.00021144834,0.71529573,0.020297274,0.0021842513,0.008464978,0.00007161365],"about_ca_topic_score_codex":0.011775601,"about_ca_topic_score_gemma":0.011699409,"teacher_disagreement_score":0.011775601,"about_ca_system_score_codex":0.00048923324,"about_ca_system_score_gemma":0.0005088016,"threshold_uncertainty_score":0.023414135},"labels":[],"label_agreement":null},{"id":"W4396514813","doi":"10.3847/1538-4357/ad37fa","title":"Photon Rings and Shadow Size for General Axisymmetric and Stationary Integrable Spacetimes","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Ontario Ministry of Economic Development, Job Creation and Trade","keywords":"Shadow (psychology); Integrable system; Rotational symmetry; Photon; Physics; Classical mechanics; Mathematical physics; Optics; Mechanics; Psychology","score_opus":0.009639950492453407,"score_gpt":0.2415702996263651,"score_spread":0.23193034913391167,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396514813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96781117,0.0001300025,0.028136496,0.00008897172,0.0000035379653,0.0000059384797,0.00010571196,0.00003584085,0.0036823757],"genre_scores_gemma":[0.997809,0.00004086385,0.0019744937,0.0000034823427,0.0000050405747,0.0000024341152,0.000030708467,0.000003977996,0.00013002218],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99975365,0.00009946636,0.000014261785,0.00005501511,0.000046464174,0.000031132604],"domain_scores_gemma":[0.9964216,0.0016352875,0.0011898219,0.00036572127,0.00018249103,0.00020512326],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012920309,0.00023708762,0.00022948877,0.0010473372,0.0003148576,0.0006466968,0.00047301897,0.0002538493,0.0014219189],"category_scores_gemma":[0.0045498554,0.0001373984,0.00020887193,0.00037815722,0.0017755218,0.0012610495,0.0007462732,0.00030237404,0.000052423013],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016377232,0.00002558717,0.04061046,0.000098987955,0.000040840012,0.0005537103,0.00081359176,0.04841851,0.022398364,0.87578803,0.0004641559,0.01062398],"study_design_scores_gemma":[0.000042310694,0.00011318514,0.11983911,0.000039361967,0.000029260289,0.0011061506,0.00073018327,0.4100417,0.00911743,0.45713106,0.0017055009,0.00010483489],"about_ca_topic_score_codex":0.00075089623,"about_ca_topic_score_gemma":0.0005365599,"teacher_disagreement_score":0.0014219189,"about_ca_system_score_codex":0.0004872088,"about_ca_system_score_gemma":0.00013739053,"threshold_uncertainty_score":0.006833017},"labels":[],"label_agreement":null},{"id":"W4396579115","doi":"10.3847/1538-4357/ad3042","title":"SAGAbg. I. A Near-unity Mass-loading Factor in Low-mass Galaxies via Their Low-redshift Evolution in Stellar Mass, Oxygen Abundance, and Star Formation Rate","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; University of Edinburgh; Integrated Electronics Engineering Center, Binghamton University; Smithsonian Astrophysical Observatory; York University; Ministério da Ciência, Tecnologia e Inovação; Science and Technology Facilities Council; Office of Science; University of Colorado Boulder; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astrophysik; University of Sussex; Institut de Física d'Altes Energies; Universidad Nacional Autónoma de México; U.S. Department of Energy; Yale University; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Deutsche Forschungsgemeinschaft; Chinese Academy of Sciences; High Energy Physics; Fermilab; Max-Planck-Institut für Astronomie; University of Nottingham; University of Oxford; Instituto de Astrofísica de Canarias; University of Cambridge; Leibniz-Gemeinschaft; National Science Foundation; University of Michigan; University of Notre Dame; National Aeronautics and Space Administration; University College London; Carnegie Mellon University; University of Washington; Johns Hopkins University; Vanderbilt University; University of Chicago; Ohio State University; Carnegie Institution of Washington; New Mexico State University; University of Portsmouth; Smithsonian Institution; California Institute of Technology; Division of Astronomical Sciences; Financiadora de Estudos e Projetos; University of Pennsylvania","keywords":"Astrophysics; Physics; Redshift; Stellar mass; Galaxy; Star formation; Metallicity; Galaxy formation and evolution","score_opus":0.0071679751691208615,"score_gpt":0.20524244481798637,"score_spread":0.19807446964886552,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396579115","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99424344,0.000051272953,0.0019763303,0.00005268766,0.000003820203,0.0000074624304,0.0014015563,0.0002741991,0.0019891628],"genre_scores_gemma":[0.9971813,0.000010749105,0.00096112996,0.000017812983,0.0000022780662,0.0000040259856,0.0014479946,0.000022928712,0.0003518426],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983525,0.000025380135,0.000009678241,0.00005839505,0.00002997272,0.0000414062],"domain_scores_gemma":[0.9991454,0.00013359028,0.00028690175,0.0001579475,0.000106475876,0.00016961849],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003546363,0.00023114165,0.00021152102,0.00089808786,0.00028664275,0.0008309476,0.00021800892,0.00024543313,0.003089595],"category_scores_gemma":[0.0010439364,0.00015223351,0.00028787766,0.000800421,0.0002959958,0.00027702522,0.00045459814,0.00019869734,0.00087897823],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000071283,0.00001565178,0.98528385,0.000016465727,0.000030639378,0.000049516202,0.000060287344,0.00064957625,0.0052192435,0.00045841126,0.0005160509,0.007629059],"study_design_scores_gemma":[0.000005316991,0.000028062097,0.99126256,0.000004364496,0.000021134842,0.00010016575,0.00008306829,0.0043922113,0.0027443327,0.00042932655,0.0009262683,0.0000030971912],"about_ca_topic_score_codex":0.005086809,"about_ca_topic_score_gemma":0.0043785665,"teacher_disagreement_score":0.005086809,"about_ca_system_score_codex":0.00029116677,"about_ca_system_score_gemma":0.00012133519,"threshold_uncertainty_score":0.010335743},"labels":[],"label_agreement":null},{"id":"W4396582754","doi":"10.3847/1538-4357/ad2ae7","title":"The Next Generation Virgo Cluster Survey. XXXVII. Distant RR Lyrae Stars and the Milky Way Stellar Halo Out to 300 kpc","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"National Science Foundation","keywords":"RR Lyrae variable; Physics; Astrophysics; Milky Way; Globular cluster; Galactic halo; Astronomy; Halo; Metallicity; Stars; Galaxy","score_opus":0.025800500068671583,"score_gpt":0.24431563333839518,"score_spread":0.2185151332697236,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396582754","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5656871,0.0033142234,0.0015602765,0.0016349001,0.0001873315,0.00020272486,0.39988542,0.0016991583,0.025828896],"genre_scores_gemma":[0.57943076,0.0013545826,0.00426897,0.0007914672,0.00016363812,0.00021652547,0.38113284,0.00041806986,0.03222315],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998666,0.000013917248,0.000008698259,0.00003725024,0.00003803641,0.000035531553],"domain_scores_gemma":[0.9996014,0.000019198951,0.00007120464,0.000064345026,0.00007113852,0.00017270917],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003630053,0.0002251519,0.00019359287,0.0018791239,0.00028391692,0.00067429716,0.0003660427,0.00027234099,0.005155234],"category_scores_gemma":[0.0005558867,0.00014801155,0.00035268985,0.0017542394,0.00008575833,0.00024145092,0.0008749006,0.00021440495,0.0037999123],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034591666,0.00006671938,0.81107223,0.00022266027,0.00018331243,0.00031636914,0.00040842546,0.00089119334,0.0041803923,0.0009831616,0.1290664,0.0522632],"study_design_scores_gemma":[0.0000120153745,0.000008994578,0.9723461,0.000012587814,0.000019119401,0.00006571715,0.000054275395,0.00020788432,0.00019801078,0.000070558424,0.02699956,0.0000051663733],"about_ca_topic_score_codex":0.07632362,"about_ca_topic_score_gemma":0.089820564,"teacher_disagreement_score":0.07632362,"about_ca_system_score_codex":0.00065176806,"about_ca_system_score_gemma":0.00048338695,"threshold_uncertainty_score":0.15175873},"labels":[],"label_agreement":null},{"id":"W4396612154","doi":"10.3847/1538-4357/ad343c","title":"Unveiling the Small-scale Jets in the Rapidly Growing Supermassive Black Hole IZw1","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"National Key Research and Development Program of China; Science and Technology Facilities Council; China Postdoctoral Science Foundation; National Natural Science Foundation of China; European Space Agency; Grantová Agentura České Republiky; Alexander von Humboldt-Stiftung; National Science Foundation","keywords":"Physics; Astrophysics; Supermassive black hole; Active galactic nucleus; Accretion (finance); Astronomy; Black hole (networking); Astrophysical jet; Brightness; Jet (fluid); Very-long-baseline interferometry; Galaxy","score_opus":0.016378507762048775,"score_gpt":0.23992371700541687,"score_spread":0.2235452092433681,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396612154","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994215,0.00010360551,0.00022589936,0.000015473901,0.0000019851143,0.000003478035,0.00003936046,0.000007899001,0.00018081174],"genre_scores_gemma":[0.99933666,0.000051455758,0.00038527578,0.000015785403,0.000006814775,0.000003065631,0.00007811468,0.000003540547,0.000119215554],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999639,0.0000025372933,0.0000018202469,0.0000102706,0.0000065780246,0.000014972022],"domain_scores_gemma":[0.99982625,0.000015599913,0.00010035756,0.000009914131,0.000011752456,0.000036074045],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015601776,0.00019135959,0.00016613824,0.00063118024,0.00026922903,0.00038805592,0.00023237598,0.00024000336,0.0005910804],"category_scores_gemma":[0.00019448982,0.00013307823,0.00013421022,0.00022725084,0.0002308538,0.00031025536,0.0004766649,0.0003448703,0.00010562932],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025848765,0.00008855896,0.38007578,0.000059658953,0.00006370383,0.0027141846,0.00082457514,0.00056681084,0.60016483,0.00060948805,0.00025217683,0.014321735],"study_design_scores_gemma":[0.000011112409,0.00013144746,0.9894755,0.00000725132,0.00002270014,0.0006620845,0.00032113222,0.0014746211,0.007001858,0.00022962633,0.00065430923,0.000008301059],"about_ca_topic_score_codex":0.0013194211,"about_ca_topic_score_gemma":0.0025559512,"teacher_disagreement_score":0.0013194211,"about_ca_system_score_codex":0.0001562086,"about_ca_system_score_gemma":0.00008169613,"threshold_uncertainty_score":0.0026234388},"labels":[],"label_agreement":null},{"id":"W4396624364","doi":"10.3847/1538-4357/ad3444","title":"The Next Generation Virgo Cluster Survey (NGVS). XXVII. The Size and Structure of Globular Cluster Systems and Their Connection to Dark Matter Halos","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Brookhaven National Laboratory; Office of Science; Agencia Nacional de Investigación y Desarrollo; Centre National de la Recherche Scientifique; U.S. Department of Energy; National Natural Science Foundation of China; York University; Space Telescope Science Institute; Ohio State University; Higher Education Discipline Innovation Project; National Research Foundation; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Fondo Nacional de Desarrollo Científico y Tecnológico; Harvard University; Yale University; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Research Foundation of Korea; New Mexico State University; University of Portsmouth; Vanderbilt University; National Science Foundation; Lawrence Berkeley National Laboratory; Ministry of Science and ICT, South Korea; Comisión Nacional de Investigación Científica y Tecnológica; National Aeronautics and Space Administration","keywords":"Physics; Globular cluster; Astrophysics; Galaxy; Dwarf galaxy; Red-giant branch; Virgo Cluster; Stellar mass; Stars; Astronomy; Galaxy cluster; Star formation","score_opus":0.010875904603024976,"score_gpt":0.21222200184696904,"score_spread":0.20134609724394406,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396624364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9371357,0.0006978577,0.00043209072,0.00028512263,0.000022497086,0.00003312672,0.05379357,0.00013522783,0.007464797],"genre_scores_gemma":[0.9176029,0.00026872515,0.00096306426,0.00007911271,0.000020054706,0.000043495624,0.076865904,0.000027837092,0.0041290056],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999021,0.00001564317,0.000004905869,0.000018514964,0.000036051882,0.000022812941],"domain_scores_gemma":[0.99975866,0.000020114898,0.00005746591,0.00002905581,0.000059103717,0.00007561911],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026267598,0.000114648996,0.00009637222,0.001360882,0.00015714036,0.00030178996,0.00023719344,0.00010396618,0.0016790736],"category_scores_gemma":[0.0005770389,0.00006032216,0.00012917034,0.0012619441,0.00008731171,0.00017406119,0.0004177144,0.000098803706,0.00055352546],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006454094,0.000010887847,0.9681429,0.000032869917,0.00003419522,0.00004043748,0.00013309423,0.00036651688,0.0009078814,0.00037231194,0.012121375,0.017772967],"study_design_scores_gemma":[0.0000018890097,0.0000034760876,0.99523336,0.000003996399,0.0000041590747,0.000020249916,0.000041359654,0.00023096937,0.000118443786,0.000048395115,0.004292273,0.0000013855564],"about_ca_topic_score_codex":0.058478188,"about_ca_topic_score_gemma":0.076656446,"teacher_disagreement_score":0.058478188,"about_ca_system_score_codex":0.00053537113,"about_ca_system_score_gemma":0.00027238877,"threshold_uncertainty_score":0.11627561},"labels":[],"label_agreement":null},{"id":"W4396707654","doi":"10.3847/1538-4357/ad36c4","title":"The Faint Satellite System of NGC 253: Insights into Low-density Environments and No Satellite Plane*","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Royal Military College of Canada; Queen's University","funders":"National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Galaxy; Satellite galaxy; Astrophysics; Satellite; Milky Way; Astronomy; Luminosity; Local Group; Dwarf galaxy; Luminosity function; Stellar mass; Star formation","score_opus":0.0036792667425268725,"score_gpt":0.18101036762627745,"score_spread":0.1773311008837506,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396707654","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998744,0.00010523777,0.00025104394,0.0000088726265,6.961465e-7,0.0000012329476,0.00014184036,0.0000071530967,0.0007398085],"genre_scores_gemma":[0.99951434,0.00002913138,0.00021632477,0.0000040736227,0.000001358989,8.397382e-7,0.00014394733,0.0000018240307,0.00008820084],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992144,0.000013001538,0.0000060473835,0.000029157896,0.000015167134,0.000015230954],"domain_scores_gemma":[0.99940574,0.000090658395,0.0001945645,0.00008645753,0.00008255548,0.00014005286],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022598209,0.00012360926,0.00018108248,0.0006995118,0.00026754328,0.00052930694,0.00019603735,0.00010358233,0.00144502],"category_scores_gemma":[0.0004772191,0.000067244044,0.000105789804,0.0006630376,0.00042468094,0.00022302476,0.0003382494,0.00010977686,0.00031099955],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000044738288,0.0000131887045,0.9781822,0.000017095796,0.00001839798,0.00016851576,0.00023728251,0.00017977782,0.016446587,0.00023103376,0.00006105029,0.004399979],"study_design_scores_gemma":[9.977545e-7,0.000029035982,0.99739707,0.0000045646975,0.0000126957975,0.0002101589,0.00024465454,0.00024741594,0.0012515261,0.00013260396,0.00046697925,0.0000021997448],"about_ca_topic_score_codex":0.005243339,"about_ca_topic_score_gemma":0.008084716,"teacher_disagreement_score":0.005243339,"about_ca_system_score_codex":0.00021585124,"about_ca_system_score_gemma":0.00017409341,"threshold_uncertainty_score":0.010425627},"labels":[],"label_agreement":null},{"id":"W4396737798","doi":"10.3847/1538-4357/ad37f6","title":"Investigating the Soft X-Ray Spectra of Solar Flare Onsets","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Aeronautics and Space Administration","keywords":"Physics; Flare; Solar flare; Astrophysics; Plasma; Spectral line; Coronal loop; Imaging spectrometer; Spectrometer; Phase (matter); Astronomy; Coronal mass ejection; Solar wind; Optics","score_opus":0.008297759158240986,"score_gpt":0.23192928208147906,"score_spread":0.22363152292323807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396737798","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969133,0.0001482006,0.0008537612,0.000019048244,0.000007254236,0.0000086007785,0.0007824749,0.000106354986,0.0011609744],"genre_scores_gemma":[0.99664414,0.00007440169,0.0009002335,0.000011763505,0.000012300979,0.000007653798,0.0019681538,0.000026951646,0.0003542942],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999299,0.000003782858,0.00000464922,0.000019580351,0.000025826084,0.000016191138],"domain_scores_gemma":[0.99979323,0.00003638648,0.000065189626,0.000017314185,0.000052850402,0.000035133075],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015423552,0.00029045754,0.0001938707,0.0014226597,0.00023020933,0.00035094426,0.00020431358,0.0002904473,0.0008299296],"category_scores_gemma":[0.00031777166,0.00011217942,0.00032929206,0.00086739147,0.00010224953,0.00028383167,0.00028567476,0.0002696264,0.00018342937],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004396327,0.00012711108,0.82242495,0.00014988006,0.00022083068,0.0013609311,0.0005705434,0.0037818141,0.1326188,0.00035195795,0.0013835523,0.03656999],"study_design_scores_gemma":[0.0000046757164,0.00002873978,0.9902058,0.00000463994,0.000020577194,0.0001894629,0.00010605074,0.0036152285,0.0046816375,0.00004573643,0.0010893337,0.000008096831],"about_ca_topic_score_codex":0.002242807,"about_ca_topic_score_gemma":0.0036909867,"teacher_disagreement_score":0.002242807,"about_ca_system_score_codex":0.00018690404,"about_ca_system_score_gemma":0.00007137993,"threshold_uncertainty_score":0.0044595003},"labels":[],"label_agreement":null},{"id":"W4396769951","doi":"10.3847/1538-4357/ad35b6","title":"The JCMT Transient Survey: Six Year Summary of 450/850 μm Protostellar Variability and Calibration Pipeline Version 2.0","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Atmospheric Ozone and Climate","field":"Earth and Planetary Sciences","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; Korea Astronomy and Space Science Institute; National Research Foundation of Korea; Academia Sinica; Canadian Space Agency; National Research Foundation; National Astronomical Research Institute of Thailand","keywords":"Transient (computer programming); Calibration; Pipeline (software); Physics; Astrophysics; Protostar; Astronomy; Remote sensing; Environmental science; Geology; Computer science; Star formation; Stars; Operating system","score_opus":0.008888038334997335,"score_gpt":0.20942098655235117,"score_spread":0.20053294821735385,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396769951","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.4349389,0.001288708,0.04409582,0.00082811323,0.00022557807,0.0013668757,0.4801823,0.023655957,0.013417684],"genre_scores_gemma":[0.32384786,0.0005334344,0.05180561,0.000535441,0.00028527263,0.0009878669,0.6127299,0.004196277,0.00507843],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99825543,0.00016619248,0.00016459999,0.00038132787,0.0008289781,0.00020347517],"domain_scores_gemma":[0.9893856,0.0006408842,0.002119159,0.0026447524,0.004205582,0.0010039941],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004217304,0.00081072527,0.00074497936,0.004733677,0.00074054266,0.0015094278,0.0013132853,0.0006571975,0.0036798234],"category_scores_gemma":[0.0061982865,0.0009182789,0.0008515559,0.00574453,0.00024856615,0.00084314274,0.0015278464,0.00065141346,0.00511828],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052614533,0.0002450489,0.7280103,0.00040086528,0.00038674596,0.00032334073,0.0007450424,0.00791234,0.01643295,0.00039539367,0.13148262,0.11313922],"study_design_scores_gemma":[0.000027715821,0.00005550123,0.9676847,0.000032301075,0.000056127832,0.0001171669,0.000055822275,0.0040339823,0.0020487816,0.00007608826,0.02577272,0.000039100894],"about_ca_topic_score_codex":0.04348985,"about_ca_topic_score_gemma":0.05504981,"teacher_disagreement_score":0.04348985,"about_ca_system_score_codex":0.0010968858,"about_ca_system_score_gemma":0.0014250103,"threshold_uncertainty_score":0.086473405},"labels":[],"label_agreement":null},{"id":"W4396788222","doi":"10.3847/1538-4357/ad4ee3","title":"Structure and Kinematics of Star-forming Elliptical Galaxies in SDSS-MaNGA","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; York University; Ministério da Ciência, Tecnologia e Inovação; Science and Technology Facilities Council; Office of Science; University of Colorado Boulder; Lawrence Berkeley National Laboratory; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Instituto de Astrofísica de Canarias; Fermilab; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Deutsche Forschungsgemeinschaft; Chinese Academy of Sciences; High Energy Physics; Department of Atomic Energy, Government of India; University of Sussex; University of Nottingham; University of Oxford; University of Chicago; National Energy Research Scientific Computing Center; Leibniz-Gemeinschaft; National Science Foundation; University of Michigan; University of Notre Dame; National Aeronautics and Space Administration; University College London; Carnegie Mellon University; University of Washington; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Portsmouth; New Mexico State University; University of Utah; Vanderbilt University; Ohio State University; Smithsonian Institution; Yale University; U.S. Department of Energy; California Institute of Technology; Division of Astronomical Sciences; Financiadora de Estudos e Projetos; University of Pennsylvania","keywords":"Astrophysics; Kinematics; Elliptical galaxy; Star (game theory); Galaxy; Physics; Astronomy; Classical mechanics","score_opus":0.01260726974703436,"score_gpt":0.2788823003629009,"score_spread":0.26627503061586655,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396788222","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979354,0.000035266436,0.00023187757,0.000021328617,0.000001887155,0.0000052326172,0.001143551,0.00008806084,0.0005373363],"genre_scores_gemma":[0.9949616,0.00001972666,0.0010821598,0.000015577652,0.0000042944857,0.0000074105105,0.0035302192,0.000029449006,0.0003496811],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981827,0.000025280468,0.0000102570075,0.00008328163,0.000025775687,0.000037180474],"domain_scores_gemma":[0.99938035,0.000078465884,0.00017664896,0.00010481888,0.000089763795,0.00016995943],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036017795,0.00020183652,0.00019605437,0.0016918386,0.0002802326,0.00043890328,0.00025570713,0.00014627178,0.0010371597],"category_scores_gemma":[0.0006209053,0.00018899216,0.00028988128,0.0006978924,0.00030107153,0.00030269567,0.0006096294,0.00013873148,0.000594402],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012418922,0.00006650153,0.97928876,0.000028075823,0.00005487452,0.000113100585,0.00048095055,0.0010830064,0.010568065,0.00035883678,0.0008024611,0.0070312237],"study_design_scores_gemma":[0.000006035087,0.000017365848,0.9949197,0.000005557085,0.000008916627,0.000058868718,0.00012749436,0.003064318,0.0008629473,0.000107474,0.0008161129,0.0000052088703],"about_ca_topic_score_codex":0.006977728,"about_ca_topic_score_gemma":0.010006478,"teacher_disagreement_score":0.006977728,"about_ca_system_score_codex":0.00043052054,"about_ca_system_score_gemma":0.00020544503,"threshold_uncertainty_score":0.013874233},"labels":[],"label_agreement":null},{"id":"W4396799416","doi":"10.3847/1538-4357/ad3643","title":"Active Galactic Nuclei Selection and Demographics: A New Age with JWST/MIRI","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":84,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Agencia Estatal de Investigación; Astrophysics Science Division; European Research Council; Goddard Space Flight Center; Jet Propulsion Laboratory","keywords":"Demographics; Selection (genetic algorithm); Astronomy; Geography; Astrophysics; Computer science; Demography; Physics; Sociology; Artificial intelligence","score_opus":0.007892970862428858,"score_gpt":0.22358923758317248,"score_spread":0.21569626672074363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396799416","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9696815,0.0064480808,0.0032566078,0.0067603057,0.0001219898,0.00003274337,0.0031384823,0.00017759486,0.010382719],"genre_scores_gemma":[0.98690724,0.0025587939,0.003414316,0.0014761292,0.00043746128,0.000027929102,0.002513116,0.00013836335,0.002526675],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993137,0.000107922,0.000055875844,0.00023883085,0.0001992386,0.000084443505],"domain_scores_gemma":[0.9939323,0.0010494161,0.0022531531,0.00084434607,0.00090932363,0.0010114458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020282054,0.00014357221,0.0003183226,0.0015497966,0.00037032197,0.0014578918,0.0006264368,0.00044014998,0.0024830846],"category_scores_gemma":[0.0067544524,0.00015783159,0.00019039208,0.0017142441,0.00069515,0.002762631,0.0013189417,0.0008927947,0.00064763275],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006303934,0.000030364581,0.9463419,0.000025179055,0.000028266704,0.00014215324,0.0006823278,0.00005597304,0.001414474,0.0009678637,0.0036009233,0.046647575],"study_design_scores_gemma":[0.0000025159386,0.00004261203,0.9866702,0.000050594306,0.000018099148,0.00083375897,0.0005523884,0.00039071107,0.0004360938,0.00105984,0.009930705,0.000012497413],"about_ca_topic_score_codex":0.0023667454,"about_ca_topic_score_gemma":0.00542709,"teacher_disagreement_score":0.0024830846,"about_ca_system_score_codex":0.00033460697,"about_ca_system_score_gemma":0.0003156484,"threshold_uncertainty_score":0.010726333},"labels":[],"label_agreement":null},{"id":"W4396804364","doi":"10.3847/1538-4357/ad35bd","title":"X-Ray and Radio Monitoring of the Neutron Star Low-mass X-Ray Binary 1A 1744-361: Quasiperiodic Oscillations, Transient Ejections, and a Disk Atmosphere","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Astrophysics Division; Astrophysics Science Division; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; Japan Aerospace Exploration Agency; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; National Research Foundation; University of Leicester; University of Warwick; RIKEN; National Aeronautics and Space Administration; Goddard Space Flight Center","keywords":"Physics; Astrophysics; Ejecta; Neutron star; Low Mass; Accretion (finance); Astronomy; Quasiperiodic function; Flare; Stars; Supernova","score_opus":0.008178994111281769,"score_gpt":0.21970767593939525,"score_spread":0.2115286818281135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396804364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99955755,0.000037744547,0.000042050982,0.0000095927435,0.0000022012953,0.0000040671216,0.00008056694,0.0000035969945,0.00026260168],"genre_scores_gemma":[0.99901056,0.000032165473,0.00026194387,0.00001522322,0.0000125613915,0.000004080518,0.0004441956,0.0000034693649,0.00021586115],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999101,0.0000121202465,0.000006010569,0.00002623259,0.000025924179,0.00001964361],"domain_scores_gemma":[0.9996685,0.000038232185,0.00011393468,0.000026521027,0.000053959127,0.00009885976],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022453471,0.0002038454,0.00026232735,0.00095393567,0.0005973977,0.00033353243,0.00020734525,0.00019498689,0.00047997275],"category_scores_gemma":[0.0003154411,0.000109540124,0.00012645323,0.00045991535,0.0001911251,0.00016676675,0.00043126426,0.00023736195,0.0001772648],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000576005,0.00016688865,0.89224017,0.000041793886,0.00006695832,0.0025191857,0.0005447359,0.00040226438,0.09221752,0.00009868005,0.0003065705,0.010819295],"study_design_scores_gemma":[0.0000056011017,0.000107226144,0.99754375,0.000002115222,0.000010354246,0.00033638487,0.000109060114,0.00024437965,0.0012366348,0.000014164011,0.0003862194,0.000004060639],"about_ca_topic_score_codex":0.0036433912,"about_ca_topic_score_gemma":0.008325229,"teacher_disagreement_score":0.0036433912,"about_ca_system_score_codex":0.00030738884,"about_ca_system_score_gemma":0.00014262431,"threshold_uncertainty_score":0.0072443485},"labels":[],"label_agreement":null},{"id":"W4396804396","doi":"10.3847/1538-4357/ad3631","title":"The Mass Dependence of Hα Emission and Stellar Spindown for Fully Convective M Dwarfs","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Convection; Astrophysics; Physics; Stars; Astronomy; Meteorology","score_opus":0.00952429404559382,"score_gpt":0.24093670826682612,"score_spread":0.2314124142212323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396804396","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997806,0.000016695361,0.00005846268,0.0000019698327,2.8093373e-7,4.762451e-7,0.000025772357,0.000002188468,0.000113523674],"genre_scores_gemma":[0.99988437,0.000004352147,0.000031700838,0.0000015187102,8.118038e-7,3.3609604e-7,0.000049582944,9.993131e-7,0.000026321226],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999001,0.000012226081,0.000009186748,0.00003471807,0.00001852803,0.000025238718],"domain_scores_gemma":[0.9989869,0.00025930285,0.00033240317,0.0000832165,0.00010124797,0.00023692276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003081591,0.00014676747,0.00015292341,0.0009065588,0.00029760046,0.00046814553,0.00018716407,0.00022764989,0.0006500423],"category_scores_gemma":[0.0010854086,0.00011847395,0.0001387246,0.00031287104,0.00031033525,0.00025281074,0.0004093134,0.00014510777,0.00021364949],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014387167,0.000011944244,0.9835255,0.0000039798065,0.00001181367,0.000045379205,0.00011056153,0.00011314425,0.014787871,0.00005004812,0.000020314355,0.0011756067],"study_design_scores_gemma":[0.0000011175523,0.000023291179,0.9985085,7.989818e-7,0.0000029956718,0.00009296174,0.00005022386,0.00041692454,0.0008487583,0.00002799271,0.00002530419,0.0000010849138],"about_ca_topic_score_codex":0.0014287967,"about_ca_topic_score_gemma":0.0022696534,"teacher_disagreement_score":0.0014287967,"about_ca_system_score_codex":0.00018554958,"about_ca_system_score_gemma":0.000055656976,"threshold_uncertainty_score":0.0028409362},"labels":[],"label_agreement":null},{"id":"W4396813567","doi":"10.3847/1538-4357/ad488a","title":"Large-scale Overdensity of Lyman Break Galaxies around the z = 6.3 Ultraluminous Quasar J0100 + 2802","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Quasar; Galaxy; Redshift; Dark matter; Halo; Astronomy; Galaxy formation and evolution; Universe","score_opus":0.00853138495874356,"score_gpt":0.22355924051376114,"score_spread":0.21502785555501758,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396813567","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994448,0.000046504116,0.00006275611,0.000009358925,8.205705e-7,0.0000010089436,0.00012902076,0.000007970118,0.00029772668],"genre_scores_gemma":[0.9994722,0.000022019565,0.00005774953,0.0000057413436,0.000003290367,0.00000111804,0.00033721566,0.0000019406448,0.00009864975],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986947,0.000011884294,0.0000066608227,0.000039774477,0.00003634808,0.000035812755],"domain_scores_gemma":[0.99935395,0.00007722966,0.00025444955,0.000041630425,0.000070787784,0.00020201829],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017339809,0.00013980994,0.00020484511,0.0015432546,0.00035728316,0.0006274081,0.0002880921,0.00015830016,0.0015892953],"category_scores_gemma":[0.00043120465,0.00014035881,0.00015189464,0.0006262545,0.00030770316,0.00023316676,0.00052979175,0.00015319619,0.00022444119],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000052556916,0.000026717076,0.99136204,0.0000056930935,0.000022954242,0.00009563648,0.00014421203,0.00012349304,0.006023121,0.000112389695,0.00016970985,0.0018614965],"study_design_scores_gemma":[0.0000010225299,0.0000061843066,0.99956745,0.0000010539335,0.0000033626952,0.000042777287,0.00006459491,0.000107492044,0.00011041191,0.000014637924,0.00007998742,0.0000010707797],"about_ca_topic_score_codex":0.006930797,"about_ca_topic_score_gemma":0.0071830167,"teacher_disagreement_score":0.006930797,"about_ca_system_score_codex":0.00025018293,"about_ca_system_score_gemma":0.000092076654,"threshold_uncertainty_score":0.013780892},"labels":[],"label_agreement":null},{"id":"W4396860397","doi":"10.3847/1538-4357/ad372f","title":"The First High-contrast Images of Near High-mass X-Ray Binaries with Keck/NIRC2","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Université de Montréal; National Aeronautics and Space Administration; California Institute of Technology; Natural Sciences and Engineering Research Council of Canada; Institut de Valorisation des Données; W. M. Keck Foundation","keywords":"Circumbinary planet; Physics; Astrophysics; Exoplanet; Brown dwarf; Astronomy; Stars; Population; Binary number; Accretion (finance)","score_opus":0.004398597763670747,"score_gpt":0.19387040267835487,"score_spread":0.18947180491468413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396860397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.990227,0.00027706334,0.0030835208,0.000043510037,0.00000881887,0.000026918526,0.0008439441,0.00013411573,0.0053551197],"genre_scores_gemma":[0.98933816,0.00007287189,0.007412368,0.00006324249,0.0000166091,0.000015907084,0.0017323345,0.00005815219,0.00129038],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998841,0.000009000517,0.000006048254,0.000028421127,0.000036571637,0.00003578286],"domain_scores_gemma":[0.9995722,0.00005719246,0.00007061451,0.000071576396,0.00009922645,0.00012904397],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028532554,0.00019611587,0.00016201058,0.0016415775,0.00044776805,0.00048151956,0.00031533017,0.00033581292,0.0023773885],"category_scores_gemma":[0.0003225389,0.0001951368,0.0001800819,0.00055158365,0.00017260053,0.0003302497,0.0006654543,0.00036864114,0.000594606],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008634986,0.00024264358,0.20152156,0.00019247516,0.00020416471,0.0012535483,0.0005057522,0.0012108299,0.7635776,0.0007171467,0.002232687,0.027478147],"study_design_scores_gemma":[0.000010464161,0.000072159004,0.96905935,0.000013870883,0.00003428502,0.000994137,0.00011799788,0.0019436602,0.025200674,0.00012511051,0.002415115,0.000013214952],"about_ca_topic_score_codex":0.0012680315,"about_ca_topic_score_gemma":0.0038736977,"teacher_disagreement_score":0.0023773885,"about_ca_system_score_codex":0.0002462211,"about_ca_system_score_gemma":0.0001269826,"threshold_uncertainty_score":0.007953167},"labels":[],"label_agreement":null},{"id":"W4396864556","doi":"10.3847/1538-4357/ad39e6","title":"Forming Mercury from Excited Initial Conditions","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Mercury (programming language); Excited state; Environmental science; Materials science; Physics; Atomic physics; Computer science","score_opus":0.01221454028998841,"score_gpt":0.2583680257168593,"score_spread":0.24615348542687088,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396864556","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98153406,0.000068279835,0.0057833954,0.00019232754,0.00005737217,0.00005404543,0.00029321417,0.00018163279,0.011835817],"genre_scores_gemma":[0.9936069,0.000039539384,0.0037403142,0.00008925382,0.000009620301,0.000035823476,0.00031063822,0.00006895797,0.0020990518],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984026,0.0000297561,0.0000050649064,0.000021378804,0.000033592358,0.000069953225],"domain_scores_gemma":[0.9994863,0.00017399625,0.000060639934,0.00008613759,0.00008029335,0.000112544374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002853367,0.00028938454,0.00047574297,0.00031401377,0.0008560071,0.0007761462,0.0007154028,0.00076972117,0.005245777],"category_scores_gemma":[0.0020446612,0.00028374753,0.000599188,0.00020893947,0.0008855682,0.0007257648,0.0011551077,0.00074501516,0.00030079094],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045212588,0.00024696087,0.023796156,0.0001521807,0.00015981532,0.0010158882,0.00053713657,0.92541844,0.014552134,0.02314518,0.0023027014,0.008221196],"study_design_scores_gemma":[0.00033992575,0.00036695125,0.0084303105,0.000030584826,0.000055389675,0.00021563517,0.00033140788,0.9688005,0.011421007,0.005956437,0.0040089404,0.000042824242],"about_ca_topic_score_codex":0.008854508,"about_ca_topic_score_gemma":0.0055184574,"teacher_disagreement_score":0.008854508,"about_ca_system_score_codex":0.0008446742,"about_ca_system_score_gemma":0.0006747057,"threshold_uncertainty_score":0.01760596},"labels":[],"label_agreement":null},{"id":"W4396885077","doi":"10.3847/1538-4357/ad2f1e","title":"The Evolution of Accreting Binaries: From Brown Dwarfs to Supermassive Black Holes","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Physics; Circumbinary planet; Astrophysics; Supermassive black hole; Accretion (finance); Mass ratio; Astronomy; Exoplanet; Brown dwarf; Planet; Stars; Galaxy","score_opus":0.010512240693756674,"score_gpt":0.23588392329735566,"score_spread":0.225371682603599,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396885077","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997744,0.00004746842,0.000020823209,0.0000075696094,3.9878861e-7,8.2773437e-7,0.000025177707,0.0000013518535,0.00012199429],"genre_scores_gemma":[0.99986625,0.000017462378,0.000024320947,0.000005024351,0.000001155603,5.179925e-7,0.000034922938,9.631614e-7,0.00004935649],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999106,0.000014946787,0.0000064590445,0.000026522946,0.0000140773145,0.000027461134],"domain_scores_gemma":[0.9994324,0.00010190645,0.00022901416,0.000030454226,0.000046372053,0.00015993897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025858096,0.00017860734,0.00021984897,0.0007386513,0.00040901187,0.0007296837,0.0002730812,0.00042116758,0.0009383449],"category_scores_gemma":[0.0007361286,0.00013475497,0.00014944359,0.0004942764,0.00032534156,0.00032945597,0.0005110258,0.00021671859,0.00025727932],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003525507,0.00009747183,0.9654928,0.000014338864,0.00004727466,0.00036675614,0.00032577792,0.001073298,0.028798513,0.00024338727,0.00006397591,0.003123906],"study_design_scores_gemma":[0.0000034621235,0.000040892235,0.99778336,0.0000022716943,0.000007006994,0.00019920876,0.0001611787,0.00087313924,0.00076046784,0.00009440192,0.00007198224,0.0000027803692],"about_ca_topic_score_codex":0.003103278,"about_ca_topic_score_gemma":0.0037980892,"teacher_disagreement_score":0.003103278,"about_ca_system_score_codex":0.00038285065,"about_ca_system_score_gemma":0.00013480149,"threshold_uncertainty_score":0.0061704516},"labels":[],"label_agreement":null},{"id":"W4396906845","doi":"10.3847/1538-4357/ad3823","title":"Dissipative Dark Substructure: The Consequences of Atomic Dark Matter on Milky Way Analog Subhalos","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":24,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"U.S. Department of Energy; National Science Foundation","keywords":"Physics; Astrophysics; Dark matter; Dwarf galaxy problem; Galaxy; Milky Way; Population; Cold dark matter; Dwarf galaxy; Galaxy formation and evolution; Warm dark matter; Local Group; Dark galaxy; Astronomy; Scalar field dark matter; Galaxy group; Dark energy; Cosmology","score_opus":0.008569866857221923,"score_gpt":0.23855261543767278,"score_spread":0.22998274858045087,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396906845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99891937,0.000021956823,0.00018703585,0.00006111222,0.0000035960488,0.000004396628,0.000118848104,0.00003219789,0.00065145106],"genre_scores_gemma":[0.9993693,0.000016255515,0.00023529801,0.00002658378,0.0000031176407,0.0000036614715,0.00016239533,0.000016127262,0.00016727156],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992025,0.000018169581,0.000003647478,0.00001433822,0.000011104672,0.000032409473],"domain_scores_gemma":[0.9994825,0.00014715247,0.00008645312,0.000048154216,0.000042535474,0.00019317056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023963362,0.00041123197,0.00047736874,0.0005226187,0.0005306481,0.00091217033,0.00089691626,0.00063186797,0.0015140134],"category_scores_gemma":[0.0012595154,0.00021626818,0.0005821569,0.00038500052,0.0007810891,0.00068008853,0.0010036969,0.0007566693,0.00011064873],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000589518,0.00053608546,0.13012862,0.00008360913,0.00035049248,0.0010121149,0.0004899545,0.84598494,0.009478462,0.0068258825,0.001281765,0.0032385609],"study_design_scores_gemma":[0.00015726956,0.0001883466,0.03943481,0.000013283845,0.0000574554,0.000070035625,0.00032766868,0.9554014,0.0016951212,0.0019081776,0.00071554095,0.000030839066],"about_ca_topic_score_codex":0.016813245,"about_ca_topic_score_gemma":0.010436036,"teacher_disagreement_score":0.016813245,"about_ca_system_score_codex":0.000900056,"about_ca_system_score_gemma":0.0003892391,"threshold_uncertainty_score":0.033430755},"labels":[],"label_agreement":null},{"id":"W4396931531","doi":"10.3847/1538-4357/ad3bab","title":"Exploring the Mpc Environment of the Quasar ULAS J1342+0928 at z = 7.54","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Universität Heidelberg; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; European Southern Observatory; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Quasar; Galaxy; Astrophysics; Advanced Camera for Surveys; Astronomy; Hubble space telescope","score_opus":0.020079303397001196,"score_gpt":0.20259764480180112,"score_spread":0.18251834140479992,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396931531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976981,0.000055008648,0.00025949982,0.000058517988,0.000002164345,0.0000040021723,0.00048015718,0.00008326654,0.0013592598],"genre_scores_gemma":[0.9986206,0.000026381336,0.0003987861,0.000019279805,0.0000046637774,0.0000031556967,0.00066540384,0.000017862969,0.00024387265],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999269,0.000008692847,0.0000016128804,0.000017479366,0.000013355759,0.000031917603],"domain_scores_gemma":[0.99979156,0.000028948785,0.00006524935,0.000012392457,0.00002252926,0.00007936072],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001365101,0.0002143972,0.00021695823,0.0007506454,0.00030961327,0.00054480386,0.00029767794,0.00017552469,0.0019506671],"category_scores_gemma":[0.0002779981,0.00017115226,0.00024210285,0.00045125987,0.00015713481,0.00030422845,0.00065976207,0.0002387845,0.00029183796],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026348798,0.00013407726,0.9169544,0.000048498852,0.00014610369,0.0012607905,0.00044452047,0.009000286,0.056001425,0.0011898481,0.002738513,0.011818012],"study_design_scores_gemma":[0.000011436494,0.000040561164,0.9880134,0.000004867333,0.000036638336,0.00008988784,0.00021237822,0.008284416,0.0018002902,0.0002133207,0.0012802172,0.000012568943],"about_ca_topic_score_codex":0.015426188,"about_ca_topic_score_gemma":0.01671123,"teacher_disagreement_score":0.015426188,"about_ca_system_score_codex":0.00036244717,"about_ca_system_score_gemma":0.00016086854,"threshold_uncertainty_score":0.030672789},"labels":[],"label_agreement":null},{"id":"W4396961208","doi":"10.3847/1538-4357/ad3730","title":"All-sky Search for Transient Astrophysical Neutrino Emission with 10 Years of IceCube Cascade Events","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Queen's University","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Alliance de recherche numérique du Canada; Santen; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Fonds Wetenschappelijk Onderzoek; Nvidia; Marquette University","keywords":"Physics; Neutrino; Sky; Astrophysics; Muon; Flare; Muon neutrino; Flux (metallurgy); Cascade; Solar neutrino problem; Solar neutrino; Neutrino detector; Measurements of neutrino speed; Astronomy; Neutrino oscillation; Nuclear physics","score_opus":0.01290992384874945,"score_gpt":0.25988795278516535,"score_spread":0.2469780289364159,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396961208","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9835189,0.00018720307,0.0011449318,0.000054725766,0.000012123444,0.00008838345,0.007999154,0.00014303754,0.0068515562],"genre_scores_gemma":[0.9784733,0.00008268836,0.0018914015,0.000039137223,0.000022201302,0.00005010618,0.018823808,0.000033680146,0.0005836259],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968266,0.00004139743,0.000012607792,0.0001017354,0.00007692013,0.0000847302],"domain_scores_gemma":[0.9994351,0.0001346062,0.00014830538,0.00005824473,0.00010811292,0.000115561605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063498423,0.00042802663,0.0003288472,0.0012548191,0.00045876857,0.0007257793,0.00031114666,0.00035418654,0.0024629284],"category_scores_gemma":[0.0007626016,0.00017415582,0.00040820538,0.001046143,0.0001777531,0.0003173139,0.0006492532,0.0003135178,0.00025856937],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0028189884,0.00044841657,0.9066579,0.00015064607,0.00063019805,0.0011446939,0.00024061286,0.007947665,0.045193914,0.0011967351,0.0064763315,0.027093923],"study_design_scores_gemma":[0.00015551761,0.00041037335,0.9642773,0.000025059377,0.00018845756,0.0005276936,0.0001497625,0.011791265,0.01337441,0.00030003174,0.008771545,0.000028536942],"about_ca_topic_score_codex":0.009455095,"about_ca_topic_score_gemma":0.02058346,"teacher_disagreement_score":0.009455095,"about_ca_system_score_codex":0.0006549238,"about_ca_system_score_gemma":0.00040784248,"threshold_uncertainty_score":0.01880008},"labels":[],"label_agreement":null},{"id":"W4396961913","doi":"10.3847/1538-4357/ad3c35","title":"Intrinsic Emission of PSR B1937+21 at 327 MHz","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Acoustic Wave Resonator Technologies","field":"Engineering","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Killam Trusts","keywords":"Physics; Materials science","score_opus":0.007140939680480126,"score_gpt":0.21567715157835846,"score_spread":0.20853621189787833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4396961913","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99755186,0.00023081082,0.0006803824,0.000021052765,0.0000053728363,0.000005460898,0.0002225759,0.0000677376,0.0012147429],"genre_scores_gemma":[0.9987056,0.0000886221,0.00053234864,0.000013087414,0.000007211879,0.000006698749,0.00023548442,0.0000119964425,0.00039895697],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999405,0.0000034675047,0.0000018365372,0.000017040691,0.000021833717,0.000015376521],"domain_scores_gemma":[0.9998598,0.000026776404,0.000036579742,0.000014594054,0.00002492472,0.000037241287],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000099411474,0.00017347532,0.00016561155,0.00039232406,0.0001765452,0.0001826715,0.0001733938,0.00018477751,0.0016722693],"category_scores_gemma":[0.0002123402,0.00010270265,0.000089989444,0.0002560411,0.00017640537,0.00014706656,0.00022530633,0.00022437143,0.00031274045],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016019653,0.00001904698,0.02919168,0.0000558801,0.000026145106,0.00023941598,0.0001498377,0.00019459537,0.96228963,0.00021009316,0.00030273042,0.0071607986],"study_design_scores_gemma":[0.000027038719,0.00036955345,0.7633889,0.000023560977,0.000046065834,0.0008210334,0.00021985438,0.002762689,0.22758995,0.00031319374,0.0044176076,0.00002053109],"about_ca_topic_score_codex":0.0008937875,"about_ca_topic_score_gemma":0.0013258739,"teacher_disagreement_score":0.0016722693,"about_ca_system_score_codex":0.00018870531,"about_ca_system_score_gemma":0.0000810173,"threshold_uncertainty_score":0.005594313},"labels":[],"label_agreement":null},{"id":"W4398147487","doi":"10.3847/1538-4357/ad3ae2","title":"Black Hole–Disk Interactions in Magnetically Arrested Active Galactic Nuclei: General Relativistic Magnetohydrodynamic Simulations Using a Time-dependent, Binary Metric","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto","funders":"RES’EAU-WaterNET","keywords":"Magnetohydrodynamic drive; Physics; Binary number; Metric (unit); Active galactic nucleus; Astrophysics; Black hole (networking); Binary black hole; Magnetohydrodynamics; Magnetic field; Quantum mechanics; Mathematics; Computer science; Galaxy; Gravitational wave","score_opus":0.015832493843843665,"score_gpt":0.3327966582747738,"score_spread":0.3169641644309301,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398147487","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9940228,0.000060138394,0.001534824,0.0002314564,0.00002390464,0.000022467771,0.00028177712,0.00007099678,0.0037516418],"genre_scores_gemma":[0.99725634,0.000043245334,0.0017044771,0.000065892484,0.000014261914,0.00002653314,0.00024333937,0.000031480413,0.00061446225],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999012,0.000028807804,0.0000041349913,0.000013897053,0.000014487353,0.000037433438],"domain_scores_gemma":[0.99930143,0.00032234925,0.000095297895,0.000043860466,0.00007237523,0.00016465638],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035366003,0.00051761226,0.0005984175,0.0004718571,0.0006935344,0.00090005,0.0013060438,0.0014564361,0.0018919898],"category_scores_gemma":[0.0014440902,0.0003866835,0.00075263274,0.00045022226,0.0009892003,0.00042244626,0.00086564734,0.0008829449,0.00016631401],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017491399,0.00017494602,0.008657392,0.000024417037,0.000062257204,0.00022393206,0.00009376294,0.98591274,0.001339225,0.0021081588,0.00041028988,0.0008179776],"study_design_scores_gemma":[0.000072077986,0.000043906537,0.0018193392,0.0000033260067,0.000010904527,0.000014363369,0.000051082785,0.9972096,0.00016193022,0.00044672308,0.00016027079,0.000006375712],"about_ca_topic_score_codex":0.02370928,"about_ca_topic_score_gemma":0.011979116,"teacher_disagreement_score":0.02370928,"about_ca_system_score_codex":0.0010012406,"about_ca_system_score_gemma":0.0007822131,"threshold_uncertainty_score":0.047142506},"labels":[],"label_agreement":null},{"id":"W4398168757","doi":"10.3847/1538-4357/ad3cd8","title":"eDIG-CHANGES. II. Project Design and Initial Results on NGC 3556","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Manitoba","funders":"Agencia Estatal de Investigación; National Natural Science Foundation of China; National Key Research and Development Program of China; Deutsche Forschungsgemeinschaft","keywords":"Engineering","score_opus":0.03389059824084123,"score_gpt":0.274210167924421,"score_spread":0.24031956968357976,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398168757","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9407372,0.000111066845,0.016759923,0.0003003837,0.000039621485,0.009565996,0.016934115,0.0013767076,0.0141749205],"genre_scores_gemma":[0.8306948,0.00009350846,0.10169047,0.00029753454,0.000040183637,0.00868239,0.048789892,0.0005325529,0.00917863],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9986141,0.0004271994,0.000054727458,0.00029797526,0.0002522245,0.00035377694],"domain_scores_gemma":[0.99825245,0.00012480498,0.00012639229,0.00029803018,0.00043170602,0.0007666127],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0030245995,0.00063899014,0.0002727994,0.00047146954,0.000795205,0.00059228524,0.0008437619,0.00059701124,0.003353434],"category_scores_gemma":[0.0012370581,0.00029080058,0.00031385274,0.0003875733,0.00039346135,0.00040732473,0.0015437073,0.00041202875,0.0015755893],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.01992293,0.01063321,0.39718962,0.00078003807,0.00024657566,0.002446694,0.0035814403,0.027631968,0.25626725,0.004450722,0.024581298,0.25226828],"study_design_scores_gemma":[0.005745031,0.022273894,0.6787036,0.00010710833,0.00023232974,0.0010207141,0.0028646993,0.02021785,0.15540068,0.001608777,0.111677594,0.00014772058],"about_ca_topic_score_codex":0.007435939,"about_ca_topic_score_gemma":0.011765356,"teacher_disagreement_score":0.007435939,"about_ca_system_score_codex":0.0009393843,"about_ca_system_score_gemma":0.0012507794,"threshold_uncertainty_score":0.01599574},"labels":[],"label_agreement":null},{"id":"W4398168763","doi":"10.3847/1538-4357/ad3d51","title":"Dynamics of Star Cluster Formation: Mergers in Gas-rich Environments","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Cluster (spacecraft); Astrophysics; Star (game theory); Astrobiology; Star cluster; Astronomy; Dynamics (music); Economic geography; Physics; Geography; Computer science; Stars; Computer network","score_opus":0.006782165510894881,"score_gpt":0.22427389072526988,"score_spread":0.217491725214375,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398168763","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966524,0.00005103954,0.0008487401,0.0001683771,0.000012283133,0.000015540654,0.00013593603,0.00005425276,0.0020614446],"genre_scores_gemma":[0.9987937,0.00003178265,0.0007117401,0.000045396304,0.0000067590863,0.000008566552,0.00013255305,0.000020953508,0.00024849648],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99979705,0.00005105469,0.000007779215,0.000038631053,0.000035762514,0.00006980585],"domain_scores_gemma":[0.99921036,0.00025795135,0.00011183517,0.000058995527,0.0000842754,0.00027646232],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005879211,0.00044813872,0.0006145656,0.0005069026,0.0010549532,0.0012616033,0.0011087322,0.0010958778,0.0015785679],"category_scores_gemma":[0.002316599,0.00044965948,0.00061597273,0.00058418064,0.0014491341,0.0009904512,0.0010719835,0.0010302569,0.00015439841],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023905087,0.00019883932,0.020841373,0.000025299069,0.00009017388,0.00023519149,0.00018820935,0.969981,0.004324716,0.0025019536,0.00050892454,0.00086523226],"study_design_scores_gemma":[0.00011388315,0.000085711385,0.008352946,0.000005605322,0.000016880533,0.00003293325,0.000096853815,0.98950213,0.00082930294,0.0006800565,0.0002660927,0.000017644177],"about_ca_topic_score_codex":0.03607075,"about_ca_topic_score_gemma":0.019370897,"teacher_disagreement_score":0.03607075,"about_ca_system_score_codex":0.0016736311,"about_ca_system_score_gemma":0.00122374,"threshold_uncertainty_score":0.07172161},"labels":[],"label_agreement":null},{"id":"W4398177271","doi":"10.3847/1538-4357/ad354b","title":"Spectroscopic Constraints on the Mid-infrared Attenuation Curve. I. Attenuation Model Using Polycyclic Aromatic Hydrocarbon Emission","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Attenuation; Polycyclic aromatic hydrocarbon; Hydrocarbon; Infrared; Aromatic hydrocarbon; Analytical Chemistry (journal); Materials science; Chemistry; Environmental chemistry; Physics; Optics; Organic chemistry","score_opus":0.02288514504566425,"score_gpt":0.2833167338575494,"score_spread":0.26043158881188516,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398177271","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7869294,0.00044973232,0.20226267,0.00035369326,0.000015417461,0.000063150546,0.000645957,0.0005977552,0.008682266],"genre_scores_gemma":[0.9936087,0.0000804641,0.0055742953,0.00004620576,0.000009021281,0.000024529962,0.00020121368,0.000026962229,0.0004286079],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997255,0.00004080793,0.000011244839,0.00010109022,0.00007066252,0.000050692128],"domain_scores_gemma":[0.99924695,0.000164167,0.00027077098,0.00016246684,0.0000935556,0.000062143175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005814479,0.0007675133,0.0002965367,0.0006975606,0.00036342168,0.00071280054,0.0016741491,0.00077478867,0.0011531767],"category_scores_gemma":[0.0013091804,0.00034460064,0.0006093563,0.0003424325,0.000719698,0.001334141,0.0008020255,0.0005993659,0.0005537946],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027511956,0.00031163509,0.25609678,0.00016170653,0.0001499723,0.00035035165,0.00029997132,0.57265776,0.096861534,0.039635774,0.0012202804,0.031979065],"study_design_scores_gemma":[0.000028055294,0.00010966288,0.051090993,0.000018761946,0.00003401399,0.0001783702,0.000066251174,0.9292247,0.006954256,0.010519778,0.001743581,0.000031480307],"about_ca_topic_score_codex":0.006177777,"about_ca_topic_score_gemma":0.0038946616,"teacher_disagreement_score":0.006177777,"about_ca_system_score_codex":0.001054592,"about_ca_system_score_gemma":0.000368489,"threshold_uncertainty_score":0.012283623},"labels":[],"label_agreement":null},{"id":"W4398222153","doi":"10.3847/1538-4357/ad380b","title":"Abundances of Neutron-capture Elements in 62 Stars in the Globular Cluster Messier 15","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Institute of General Medical Sciences; Directorate for Mathematical and Physical Sciences; National Institutes of Health; National Science Foundation","keywords":"Physics; Astrophysics; Globular cluster; Stars; Neutron star; r-process; Nucleosynthesis; Neutron capture; s-process; Blue straggler; Astronomy; Neutron; Nuclear physics","score_opus":0.00893759276594068,"score_gpt":0.24297006411024524,"score_spread":0.23403247134430455,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398222153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995103,0.000034386354,0.000030221488,0.0000036262586,5.256254e-7,0.0000015002862,0.00013571445,0.000006175678,0.0002775959],"genre_scores_gemma":[0.99866927,0.000022849115,0.00018557049,0.000007525072,0.0000015054119,0.0000021175965,0.0006871975,0.000004057049,0.0004198325],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984634,0.0000069262633,0.000011616766,0.00006922258,0.000039468407,0.000026477752],"domain_scores_gemma":[0.99983,0.000014096653,0.000060199116,0.000013527638,0.000028673263,0.000053391323],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016466725,0.00032822703,0.00022298309,0.0018877554,0.00036651723,0.00046099312,0.00024168403,0.00023692784,0.0009143814],"category_scores_gemma":[0.00026425195,0.000099299956,0.0001966681,0.00066399,0.00023922934,0.00013569923,0.00048602253,0.00007136632,0.00038855732],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018813997,0.000015230962,0.9450634,0.00001638341,0.00008003509,0.00019747045,0.00039382835,0.00037756015,0.048329044,0.00018203424,0.00015368531,0.005003045],"study_design_scores_gemma":[0.0000034214302,0.00003391221,0.9968514,0.0000017628026,0.000008797914,0.00006243027,0.000087317596,0.00033171606,0.0020173285,0.000027670814,0.0005708911,0.0000033253668],"about_ca_topic_score_codex":0.014882506,"about_ca_topic_score_gemma":0.020866346,"teacher_disagreement_score":0.014882506,"about_ca_system_score_codex":0.0008914974,"about_ca_system_score_gemma":0.000110833644,"threshold_uncertainty_score":0.02959174},"labels":[],"label_agreement":null},{"id":"W4398222172","doi":"10.3847/1538-4357/ad452c","title":"Measurement of Interstellar Magnetization by Synchrotron Polarization Variance","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Natural Science Foundation of China","keywords":"Magnetization; Synchrotron; Polarization (electrochemistry); Physics; Variance (accounting); Condensed matter physics; Astrophysics; Materials science; Magnetic field; Optics; Chemistry; Quantum mechanics; Physical chemistry","score_opus":0.007806359342115656,"score_gpt":0.21805117736827953,"score_spread":0.21024481802616388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398222172","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8689212,0.00051251607,0.117662124,0.00017606503,0.0000654082,0.000025315274,0.00093995384,0.000713111,0.010984458],"genre_scores_gemma":[0.9929045,0.00007858738,0.006265311,0.000020445857,0.000023207553,0.000009197478,0.00021343835,0.000026847292,0.00045848268],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997012,0.00007071878,0.000008896846,0.0000937999,0.00009324958,0.000032121596],"domain_scores_gemma":[0.9995828,0.00011425307,0.00010384681,0.000056124572,0.00010578145,0.00003715053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025004582,0.00022351673,0.00016799904,0.0008387076,0.00018731297,0.0005395799,0.0002636842,0.00021265872,0.0011958538],"category_scores_gemma":[0.0010198666,0.00014186853,0.00010760004,0.0006355843,0.00027674515,0.00039802465,0.0004638335,0.00042377226,0.0003320815],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046620754,0.00008083348,0.10225308,0.000095835814,0.0001425798,0.00019643804,0.00016491885,0.0042894143,0.7869457,0.0066979965,0.001614451,0.09705256],"study_design_scores_gemma":[0.00004924095,0.00021939313,0.22821324,0.000030624215,0.000077099336,0.00080873916,0.00015301058,0.08513054,0.6725148,0.007527754,0.005193058,0.00008252923],"about_ca_topic_score_codex":0.0002771206,"about_ca_topic_score_gemma":0.00033271368,"teacher_disagreement_score":0.0011958538,"about_ca_system_score_codex":0.00019382317,"about_ca_system_score_gemma":0.00009569748,"threshold_uncertainty_score":0.004000485},"labels":[],"label_agreement":null},{"id":"W4398781028","doi":"10.3847/1538-4357/ad3e5f","title":"Mercury’s Chaotic Secular Evolution as a Subdiffusive Process","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Mercury (programming language); Chaotic; Statistical physics; Environmental science; Physics; Computer science; Artificial intelligence","score_opus":0.004376741756787336,"score_gpt":0.2529196356702383,"score_spread":0.24854289391345094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4398781028","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9820467,0.00006516833,0.013624149,0.0004931172,0.000016619928,0.000008749446,0.00005900869,0.00011479086,0.0035716896],"genre_scores_gemma":[0.99908996,0.00002463296,0.00045268855,0.000020945714,0.000003722253,0.0000032833798,0.000013687105,0.000010183253,0.0003808686],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999331,0.000015952426,0.000002762228,0.000019520974,0.000010580293,0.000018013294],"domain_scores_gemma":[0.9996848,0.00007951489,0.000091331516,0.000048063383,0.000026191985,0.00007018182],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025359023,0.0002950927,0.0003381749,0.0003343229,0.00050648913,0.0007407329,0.000578982,0.0006389691,0.0013814811],"category_scores_gemma":[0.0011582981,0.00015474847,0.0004119319,0.0002036422,0.00096721447,0.001144185,0.00074975326,0.00052575016,0.00011040496],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008016728,0.00004813789,0.022768784,0.00003613771,0.00006344869,0.0005336813,0.0004950196,0.89211017,0.016835338,0.062008377,0.0011366237,0.0038841492],"study_design_scores_gemma":[0.000013776237,0.000020338864,0.003741425,0.000004106368,0.000006204104,0.00004925304,0.000045042485,0.98744303,0.0005755659,0.0077352272,0.00035607503,0.000010009541],"about_ca_topic_score_codex":0.0107025495,"about_ca_topic_score_gemma":0.004008915,"teacher_disagreement_score":0.0107025495,"about_ca_system_score_codex":0.0009975634,"about_ca_system_score_gemma":0.00038317783,"threshold_uncertainty_score":0.021280527},"labels":[],"label_agreement":null},{"id":"W4399102990","doi":"10.3847/1538-4357/ad3de6","title":"Hidden Gems on a Ring: Infant Massive Clusters and Their Formation Timeline Unveiled by ALMA, HST, and JWST in NGC 3351","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":26,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Astrophysics Division; National Institutes of Natural Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; Mitacs; Australian Government; Canada Research Chairs; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Agencia Estatal de Investigación; National Radio Astronomy Observatory; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Timeline; Physics; Astrophysics; Astronomy; Geography; Archaeology","score_opus":0.007131540180008737,"score_gpt":0.21371453683595257,"score_spread":0.20658299665594382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399102990","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965763,0.000057336172,0.00003389726,0.00001581884,0.0000011624619,9.702039e-7,0.000092789385,0.000004771423,0.00013555503],"genre_scores_gemma":[0.99966776,0.000021301084,0.000057559573,0.0000027729006,0.0000029705334,8.5332823e-7,0.000193129,0.0000016887909,0.00005191893],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998739,0.000012369815,0.0000071464597,0.000042285585,0.000025551655,0.000038829643],"domain_scores_gemma":[0.9990196,0.00011379927,0.00039638416,0.000080213234,0.00009706496,0.00029292275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031291132,0.00013805095,0.00018808074,0.0013740315,0.0004326651,0.0007460681,0.00029082,0.00020879945,0.0008249187],"category_scores_gemma":[0.001094581,0.00012893419,0.00014664646,0.00078668783,0.00032255088,0.0004715158,0.00073790277,0.00026207187,0.00019428818],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001037598,0.000015844924,0.9928716,0.0000056793606,0.000014882656,0.00023839381,0.0006012621,0.00015283284,0.0026526852,0.00009141335,0.00017476895,0.0030768784],"study_design_scores_gemma":[9.49067e-7,0.000010105488,0.99917835,0.000002136189,0.0000042011116,0.000065070795,0.000192669,0.00030321817,0.00012196204,0.000014945403,0.00010406032,0.0000022135496],"about_ca_topic_score_codex":0.010996345,"about_ca_topic_score_gemma":0.017071199,"teacher_disagreement_score":0.010996345,"about_ca_system_score_codex":0.00039983046,"about_ca_system_score_gemma":0.00016756948,"threshold_uncertainty_score":0.021864653},"labels":[],"label_agreement":null},{"id":"W4399117685","doi":"10.3847/1538-4357/ad3fb1","title":"Search for Synchrotron Emission from Secondary Electrons ofProton–Proton Interactions in Galactic PeVatron Candidate HESSJ1641–463","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; National Research Council Canada; University of Manitoba","funders":"","keywords":"Proton; Physics; Synchrotron; Electron; Proton Synchrotron; Astrophysics; Nuclear physics","score_opus":0.01069036886880443,"score_gpt":0.28094558570300726,"score_spread":0.27025521683420284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399117685","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982993,0.00011368416,0.00022765569,0.000027150756,0.0000045713286,0.000006493823,0.00031515214,0.000027080056,0.0009789249],"genre_scores_gemma":[0.9979048,0.000052593547,0.0004084619,0.000020403268,0.0000074460677,0.000006123105,0.0010146218,0.000010832611,0.0005746886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995077,0.000003693452,0.0000025253826,0.000016144555,0.00001119593,0.000015721764],"domain_scores_gemma":[0.9998098,0.000019767884,0.000057162695,0.000016161566,0.000025906922,0.000071233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011983659,0.00026644865,0.00025238155,0.0010556339,0.00043636496,0.0005239717,0.00022682699,0.00031936826,0.003024198],"category_scores_gemma":[0.00016146695,0.00014983198,0.0002449263,0.00057928445,0.00013132048,0.00016346642,0.00039663794,0.00017618484,0.0005129678],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006084035,0.0001138427,0.78938115,0.00013591912,0.00014301902,0.0039398163,0.0003263641,0.00054275355,0.19198862,0.0003534799,0.000993566,0.011473154],"study_design_scores_gemma":[0.000017223898,0.00012033874,0.986233,0.000010698132,0.00004709603,0.0012220809,0.000273118,0.00075412716,0.008713927,0.00010645388,0.0024892308,0.000012680996],"about_ca_topic_score_codex":0.0010212128,"about_ca_topic_score_gemma":0.0019399113,"teacher_disagreement_score":0.003024198,"about_ca_system_score_codex":0.00017770735,"about_ca_system_score_gemma":0.00010100435,"threshold_uncertainty_score":0.010116935},"labels":[],"label_agreement":null},{"id":"W4399129478","doi":"10.3847/1538-4357/ad3b95","title":"Katachi (形): Decoding the Imprints of Past Star Formation on Present-day Morphology in Galaxies with Interpretable CNNs*","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Aeronautics and Space Administration","keywords":"Morphology (biology); Star (game theory); Galaxy; Decoding methods; Astrophysics; Physics; Computer science; Biology; Zoology; Algorithm","score_opus":0.009599029568212373,"score_gpt":0.23536172410682596,"score_spread":0.22576269453861358,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399129478","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7638864,0.001450795,0.21574405,0.0015793389,0.0002658595,0.000090184454,0.0022619597,0.009769556,0.0049517676],"genre_scores_gemma":[0.94846696,0.00016589469,0.044381756,0.00030321022,0.000052195806,0.000056538072,0.0027858808,0.00013010872,0.003657302],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992347,0.000013296261,0.0000027479186,0.000031427095,0.000010224021,0.000018828145],"domain_scores_gemma":[0.999701,0.00012403745,0.000028180328,0.00006172373,0.000055822868,0.000029304778],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005733862,0.0009548668,0.0003699434,0.0003784928,0.00022043227,0.00056310964,0.0011162747,0.0006911343,0.0018249524],"category_scores_gemma":[0.0016355898,0.00042574253,0.00065998215,0.00028008837,0.00036341595,0.00068525167,0.0007259093,0.0012401332,0.00053409766],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003180487,0.00019909396,0.029652469,0.00014271575,0.00053418236,0.0001918393,0.00016517137,0.70002764,0.013973045,0.004096107,0.011621357,0.23907836],"study_design_scores_gemma":[0.000010250002,0.000028418186,0.0012141721,0.0000053602007,0.00001529448,0.000009314068,0.000010296274,0.9957176,0.0015253942,0.0011588226,0.0002997547,0.000005294828],"about_ca_topic_score_codex":0.013690547,"about_ca_topic_score_gemma":0.023714518,"teacher_disagreement_score":0.013690547,"about_ca_system_score_codex":0.00075552874,"about_ca_system_score_gemma":0.00066253764,"threshold_uncertainty_score":0.02722174},"labels":[],"label_agreement":null},{"id":"W4399141302","doi":"10.3847/1538-4357/ad3e76","title":"Autoencoding Labeled Interpolator, Inferring Parameters from Image and Image from Parameters","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Image Processing Techniques","field":"Computer Science","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Image (mathematics); Artificial intelligence; Computer science; Computer vision","score_opus":0.013159514167658232,"score_gpt":0.2692793139298648,"score_spread":0.25611979976220656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399141302","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.10942546,0.000085181506,0.88787216,0.00016984883,0.00003254033,0.00002829961,0.0001280378,0.0011393307,0.0011191635],"genre_scores_gemma":[0.76371413,0.00006807281,0.23446113,0.000059862785,0.000017877872,0.000027444949,0.0003097322,0.00016482461,0.0011769384],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998728,0.00003681674,0.0000049021614,0.000040320523,0.00002787567,0.000017208216],"domain_scores_gemma":[0.9994803,0.00022375735,0.000058550282,0.00013831802,0.0000716228,0.000027492388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007224772,0.0003479646,0.00026155415,0.00036533637,0.00017428157,0.00056054967,0.0007111775,0.0007268587,0.0013075642],"category_scores_gemma":[0.002147592,0.0003128084,0.00035746343,0.00027870774,0.00052291295,0.0007636502,0.00064334396,0.000770324,0.0003037966],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018778247,0.00008092468,0.0032947487,0.00006312634,0.000043876928,0.00012890059,0.00010307427,0.80620116,0.034916047,0.013468199,0.0010906542,0.14042148],"study_design_scores_gemma":[0.0000019789582,0.000006194176,0.00017988078,0.0000022035438,0.0000015699941,0.00001202801,0.000003868033,0.9942985,0.0038626683,0.0014388945,0.00018904038,0.0000032197295],"about_ca_topic_score_codex":0.0029134704,"about_ca_topic_score_gemma":0.00252513,"teacher_disagreement_score":0.0029134704,"about_ca_system_score_codex":0.00045217184,"about_ca_system_score_gemma":0.00047822043,"threshold_uncertainty_score":0.005793035},"labels":[],"label_agreement":null},{"id":"W4399335588","doi":"10.3847/1538-4357/ad38bb","title":"What Is the Nature of Little Red Dots and what Is Not, MIRI SMILES Edition","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":174,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación","keywords":"Physics; Algorithm; Computer science","score_opus":0.005336992576256706,"score_gpt":0.22083783767257675,"score_spread":0.21550084509632006,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399335588","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87892944,0.00760085,0.0021516392,0.016508287,0.00040400738,0.000023399842,0.00897412,0.00032988747,0.08507837],"genre_scores_gemma":[0.9832297,0.0011927439,0.0008575059,0.0010231388,0.00024343777,0.000012489255,0.0032343823,0.00016902691,0.010037519],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99929535,0.00014577396,0.000030091109,0.00017072438,0.00019089725,0.00016716812],"domain_scores_gemma":[0.99681,0.0004242124,0.0011643324,0.0003316678,0.00072185183,0.00054796995],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089652406,0.00020821833,0.00029814683,0.0016390972,0.00078251393,0.0033956892,0.0005404408,0.00051155256,0.007913646],"category_scores_gemma":[0.0038530163,0.00020079692,0.00028794544,0.0021411953,0.0010550306,0.0024742987,0.00095269043,0.0005036,0.002425805],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042599652,0.00008179429,0.7510329,0.00042571468,0.00014139178,0.00059215975,0.004890029,0.0007613629,0.0032032025,0.019574804,0.08175851,0.13711208],"study_design_scores_gemma":[0.000007413371,0.000058341164,0.8989343,0.00033438465,0.00003598421,0.00070896855,0.004982065,0.0010210773,0.0008878018,0.003731615,0.08926086,0.000037173235],"about_ca_topic_score_codex":0.008465969,"about_ca_topic_score_gemma":0.0125874495,"teacher_disagreement_score":0.008465969,"about_ca_system_score_codex":0.0008302974,"about_ca_system_score_gemma":0.0002921155,"threshold_uncertainty_score":0.02647382},"labels":[],"label_agreement":null},{"id":"W4399359948","doi":"10.3847/1538-4357/ad409c","title":"A Hubble Space Telescope Search for r-Process Nucleosynthesis in Gamma-Ray Burst Supernovae","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph","funders":"Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Northwestern University; Space Telescope Science Institute; Alfred P. Sloan Foundation; National Aeronautics and Space Administration; Research Corporation for Science Advancement; Smithsonian Institution; National Science Foundation","keywords":"Physics; Gamma-ray burst; Astrophysics; Supernova; Ejecta; Nucleosynthesis; r-process; Astronomy; Stars; Extinction (optical mineralogy)","score_opus":0.015673055990253065,"score_gpt":0.26753641953099183,"score_spread":0.2518633635407388,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399359948","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99814665,0.00008041448,0.00073987065,0.000015082352,0.0000021917115,0.0000052579385,0.00011302879,0.000031618172,0.00086594437],"genre_scores_gemma":[0.9984888,0.00003221721,0.0008730885,0.000009689277,0.000004010351,0.0000027659744,0.0002369449,0.0000024226174,0.00034990214],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.000010188946,0.0000027245653,0.000023396826,0.000012311989,0.000013918194],"domain_scores_gemma":[0.999584,0.00009363072,0.00012962632,0.000038006772,0.000050410083,0.00010431684],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037286707,0.00018796904,0.00011129126,0.00063112343,0.00018384118,0.00038609357,0.00016535861,0.00015188595,0.0013974214],"category_scores_gemma":[0.00043575434,0.000106051906,0.00014413887,0.0002856037,0.00015972403,0.00017431896,0.00021064132,0.00015989471,0.00026365602],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001785752,0.000058664544,0.8914073,0.000026161075,0.00005145433,0.00021411538,0.00008905999,0.0005702995,0.0990957,0.00034378294,0.00013006189,0.007834881],"study_design_scores_gemma":[0.000004915148,0.000079259546,0.992284,0.0000033993936,0.000013666517,0.00015949208,0.00003741286,0.0014775703,0.0054379385,0.00012463926,0.00037493207,0.0000026728903],"about_ca_topic_score_codex":0.0017002814,"about_ca_topic_score_gemma":0.0026979707,"teacher_disagreement_score":0.0017002814,"about_ca_system_score_codex":0.00023208481,"about_ca_system_score_gemma":0.00012780109,"threshold_uncertainty_score":0.004674852},"labels":[],"label_agreement":null},{"id":"W4399364202","doi":"10.3847/1538-4357/ad39e5","title":"PHANGS-ML: Dissecting Multiphase Gas and Dust in Nearby Galaxies Using Machine Learning","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Alberta","funders":"Smithsonian Astrophysical Observatory; Agencia Nacional de Investigación y Desarrollo; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Agence Nationale de la Recherche; National Science Foundation","keywords":"Galaxy; Astrophysics; Environmental science; Computer science; Artificial intelligence; Physics","score_opus":0.015201709020603171,"score_gpt":0.2604941653467969,"score_spread":0.24529245632619376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399364202","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93361104,0.00046627576,0.051333178,0.00047097297,0.000045871115,0.00008226321,0.0056513986,0.0064893323,0.0018497029],"genre_scores_gemma":[0.943052,0.00006153151,0.050744697,0.00009542073,0.000079282014,0.00004117437,0.0052120816,0.00020083606,0.00051295286],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997197,0.000082200495,0.000014673393,0.00008722902,0.00005411996,0.000042126],"domain_scores_gemma":[0.9990171,0.000344816,0.00021190676,0.00018528086,0.000073239025,0.00016769761],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008932111,0.00041636708,0.00039271417,0.0023721647,0.0004681542,0.0009328626,0.0008956357,0.0005424106,0.0011935721],"category_scores_gemma":[0.0014929781,0.0001957038,0.00071661576,0.0010598066,0.00037283133,0.00061772735,0.00087279914,0.00050690403,0.0006379134],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053015864,0.0007509807,0.67822725,0.00022461585,0.0006908521,0.0007869722,0.000769797,0.08742585,0.0510111,0.0029231843,0.013579933,0.16307941],"study_design_scores_gemma":[0.00008651147,0.00012579327,0.32498008,0.00003556815,0.000057984143,0.00016065685,0.00052487926,0.6551651,0.0073949243,0.006746014,0.0046712635,0.000051185325],"about_ca_topic_score_codex":0.0042061666,"about_ca_topic_score_gemma":0.0060555125,"teacher_disagreement_score":0.0042061666,"about_ca_system_score_codex":0.0003552609,"about_ca_system_score_gemma":0.00033483194,"threshold_uncertainty_score":0.008363366},"labels":[],"label_agreement":null},{"id":"W4399364238","doi":"10.3847/1538-4357/ad3a52","title":"Chemical Diversity on Small Scales: Abundance Analysis of the Tucana V Ultrafaint Dwarf Galaxy","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Vetenskapsrådet","keywords":"Dwarf galaxy; Abundance (ecology); Astrophysics; Dwarf spheroidal galaxy; Galaxy; Physics; Biology; Ecology; Interacting galaxy","score_opus":0.011589954661062711,"score_gpt":0.21530015083997014,"score_spread":0.20371019617890743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399364238","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985935,0.00014862546,0.00009831528,0.000013936839,0.0000016362433,0.0000032737958,0.00029128298,0.000014134028,0.0008351819],"genre_scores_gemma":[0.99907255,0.000043211778,0.00017349482,0.000009333605,0.0000031431734,0.000002678768,0.00052089937,0.00000620842,0.00016857409],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998437,0.0000074747645,0.000005049408,0.000064241656,0.000036111403,0.00004339253],"domain_scores_gemma":[0.99961436,0.00004445637,0.00008304918,0.000035943063,0.00008905076,0.00013314335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014121785,0.00021190174,0.00028059835,0.0027146342,0.00072684104,0.0010230258,0.00041398924,0.0002704583,0.00069645495],"category_scores_gemma":[0.00045013448,0.000116557894,0.00018098236,0.0016212704,0.00038059754,0.00019747157,0.0006194238,0.00016165459,0.000113644135],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001918171,0.00004640341,0.9346656,0.000038517977,0.00015673494,0.00018597119,0.00069236953,0.0012585985,0.046708643,0.00042380084,0.00043556793,0.015195938],"study_design_scores_gemma":[0.0000033640772,0.000021315222,0.9954016,0.00000426206,0.000020256255,0.000067289955,0.00031511125,0.0014465916,0.001406863,0.00008119311,0.0012252828,0.0000068351796],"about_ca_topic_score_codex":0.096547134,"about_ca_topic_score_gemma":0.08419187,"teacher_disagreement_score":0.096547134,"about_ca_system_score_codex":0.0012662803,"about_ca_system_score_gemma":0.0003685099,"threshold_uncertainty_score":0.19197035},"labels":[],"label_agreement":null},{"id":"W4399384714","doi":"10.3847/1538-4357/ad40a2","title":"Evolution of the Disk in the Be Binary δ Scorpii Probed during Three Periastron Passages","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"High-pressure geophysics and materials","field":"Earth and Planetary Sciences","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Ciência sem Fronteiras; Natural Sciences and Engineering Research Council of Canada; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Fundação de Amparo à Pesquisa do Estado de São Paulo","keywords":"Binary number; Physics; Astrophysics; Mathematics; Arithmetic","score_opus":0.00862363955681327,"score_gpt":0.19974810399858225,"score_spread":0.19112446444176898,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399384714","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996934,0.000021363885,0.000036269696,0.000003828621,5.0159264e-7,0.0000011244399,0.000042403448,0.000003464886,0.00019773304],"genre_scores_gemma":[0.9996226,0.000020282063,0.000071787006,0.000003603285,8.804028e-7,0.0000015413535,0.00013867613,0.0000015375423,0.00013913978],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999615,0.0000033886274,0.0000019649801,0.0000107956275,0.000010473274,0.000011976526],"domain_scores_gemma":[0.99982554,0.000031797892,0.000054187098,0.000011732648,0.00002957731,0.000047190497],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009458998,0.00016639158,0.00018841279,0.0004995134,0.00041561024,0.00037889878,0.0001742834,0.0002968,0.0005016393],"category_scores_gemma":[0.0003905977,0.000109412766,0.00017081543,0.00032129837,0.00018611482,0.00019335673,0.0003582535,0.00022421745,0.00014645279],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047986777,0.000093337556,0.88769597,0.000045710527,0.00007679393,0.0017714939,0.0005771162,0.0039533293,0.09661882,0.00013931628,0.00011993537,0.008428322],"study_design_scores_gemma":[0.0000024919268,0.00006686723,0.995713,0.0000033276472,0.000008156691,0.00022169872,0.00014963977,0.0013860929,0.002217852,0.0000185943,0.00020845406,0.000003718002],"about_ca_topic_score_codex":0.0060032425,"about_ca_topic_score_gemma":0.008917159,"teacher_disagreement_score":0.0060032425,"about_ca_system_score_codex":0.00039142094,"about_ca_system_score_gemma":0.00010874666,"threshold_uncertainty_score":0.011936605},"labels":[],"label_agreement":null},{"id":"W4399394397","doi":"10.3847/1538-4357/ad3f17","title":"The Galaxies Missed by Hubble and ALMA: The Contribution of Extremely Red Galaxies to the Cosmic Census at 3 &lt; z &lt; 8","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":150,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Goddard Space Flight Center; Science and Technology Facilities Council; European Commission; University of Arizona; National Aeronautics and Space Administration; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Galaxy; COSMIC cancer database; Physics; Astronomy; Astrophysics","score_opus":0.008182337272586266,"score_gpt":0.21363828819227662,"score_spread":0.20545595091969035,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399394397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9923959,0.0002700105,0.0007287156,0.00040535562,0.000014444415,0.0000054368397,0.003703744,0.00014735467,0.002329154],"genre_scores_gemma":[0.9973036,0.000052754152,0.0002309557,0.00006206037,0.00001527458,0.0000031357295,0.0017794876,0.000028987139,0.0005238224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995479,0.000068344445,0.000023517434,0.00010824562,0.00016288692,0.00008912428],"domain_scores_gemma":[0.99729854,0.00039418548,0.0009678143,0.00038283656,0.00043176184,0.0005247705],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006155643,0.0001664357,0.00018662054,0.0021452,0.0002676262,0.001008257,0.000391638,0.00021690236,0.0020438342],"category_scores_gemma":[0.003149265,0.00011674187,0.00015883766,0.001139102,0.00027575588,0.0005732868,0.0005950369,0.00034344927,0.0005770383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041501393,0.000004887469,0.9886817,0.0000057127118,0.000021992195,0.000062913015,0.0001764722,0.00022648848,0.0005848545,0.0003767836,0.0015102703,0.00830652],"study_design_scores_gemma":[9.5026655e-7,0.000003094117,0.9979075,0.0000033304143,0.0000058802375,0.000049690865,0.00006036341,0.00070082536,0.00021475433,0.00010659831,0.0009439553,0.0000030354263],"about_ca_topic_score_codex":0.033290196,"about_ca_topic_score_gemma":0.042855367,"teacher_disagreement_score":0.033290196,"about_ca_system_score_codex":0.0006330865,"about_ca_system_score_gemma":0.00031498703,"threshold_uncertainty_score":0.066192865},"labels":[],"label_agreement":null},{"id":"W4399505932","doi":"10.3847/1538-4357/ad40a3","title":"Testing MOND on Small Bodies in the Remote Solar System","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Modified Newtonian dynamics; Solar System; Planetesimal; Astrophysics; Dark matter; Astronomy; Planet; Newtonian dynamics; Galactic Center; Stars; Galaxy rotation curve; Galaxy; Galaxy formation and evolution","score_opus":0.024721499175839625,"score_gpt":0.22721967371783994,"score_spread":0.2024981745420003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399505932","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99841547,0.00001838963,0.00029936736,0.000057620076,0.000004743178,0.000004097443,0.00004276039,0.000021832479,0.0011357287],"genre_scores_gemma":[0.99965405,0.0000058899454,0.00018697859,0.000010798053,0.0000018775426,0.0000020255338,0.00003953419,0.0000043303594,0.00009451417],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9998878,0.000033174976,0.0000044468675,0.000025230682,0.000018288805,0.00003110497],"domain_scores_gemma":[0.99925596,0.00038499103,0.000096627184,0.00007760038,0.000052731702,0.00013209789],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005207446,0.0003021349,0.00040623275,0.00028618044,0.0006125091,0.00047209804,0.0009065584,0.00062321423,0.0024846958],"category_scores_gemma":[0.002157229,0.00016623142,0.00047789552,0.00019488318,0.0010869168,0.0006500636,0.0010938466,0.0006486301,0.00012626383],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002959781,0.00024019789,0.052166805,0.00004418752,0.00011398029,0.0004634658,0.00023016837,0.9352653,0.0031880103,0.0041660657,0.00040393436,0.00342188],"study_design_scores_gemma":[0.00014012257,0.00033431468,0.017946368,0.000008982786,0.000025623372,0.000062362284,0.00019794668,0.97778636,0.0015547781,0.0015111377,0.00041450406,0.000017577615],"about_ca_topic_score_codex":0.0151875,"about_ca_topic_score_gemma":0.008369155,"teacher_disagreement_score":0.0151875,"about_ca_system_score_codex":0.0007545243,"about_ca_system_score_gemma":0.00034867923,"threshold_uncertainty_score":0.030198216},"labels":[],"label_agreement":null},{"id":"W4399511807","doi":"10.3847/1538-4357/ad53c5","title":"Constraining the Selection-corrected Luminosity Function and Total Pulse Count for Radio Transients","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; University of Toronto; McGill University; Ontario Power Generation; University of British Columbia","funders":"Precursory Research for Embryonic Science and Technology; Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Alliance de recherche numérique du Canada; University of Toronto; Canada Foundation for Innovation; Smithsonian Astrophysical Observatory; McGill University; Canadian Institute for Advanced Research","keywords":"Pulsar; Physics; Astrophysics; Luminosity; Luminosity function; Scaling; Algorithm; Computer science; Mathematics","score_opus":0.011581124083158303,"score_gpt":0.28735320279961335,"score_spread":0.27577207871645504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399511807","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.70607275,0.00022307079,0.29082206,0.00010876559,0.000027050386,0.000017689985,0.00031829724,0.0013052408,0.0011050971],"genre_scores_gemma":[0.95202917,0.00003743769,0.04676767,0.000032530774,0.000012311143,0.000013018036,0.0007614093,0.00012485503,0.00022169518],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955004,0.0001391249,0.000027733795,0.00016103167,0.00007856061,0.000043537362],"domain_scores_gemma":[0.9971957,0.0016728103,0.00040497456,0.00034309848,0.00025731072,0.00012598952],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026222726,0.00038026064,0.00038399326,0.00078874006,0.00036327148,0.0010524653,0.0007734092,0.0005076714,0.00084410177],"category_scores_gemma":[0.00967478,0.00032852098,0.0005832754,0.0005847895,0.0004934312,0.00081947667,0.0006336633,0.0005247011,0.0002844317],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005402649,0.00010790438,0.45865142,0.00017268906,0.00032509837,0.00031169882,0.0003746212,0.3315951,0.03519198,0.009594657,0.0015831728,0.16155136],"study_design_scores_gemma":[0.00002994551,0.00006270933,0.060533565,0.000019716303,0.000041959083,0.00017270967,0.00004980655,0.9239601,0.0092675565,0.0048748483,0.0009433274,0.000043744116],"about_ca_topic_score_codex":0.0039313403,"about_ca_topic_score_gemma":0.0030391018,"teacher_disagreement_score":0.0039313403,"about_ca_system_score_codex":0.00053975015,"about_ca_system_score_gemma":0.00067526853,"threshold_uncertainty_score":0.0138680935},"labels":[],"label_agreement":null},{"id":"W4399527845","doi":"10.3847/1538-4357/ad429e","title":"The SDSS-V Black Hole Mapper Reverberation Mapping Project: C iv Broad Absorption Line Acceleration in the Quasar SBS 1408+544","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Leibniz-Gemeinschaft; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Yunnan University; Universidad Nacional Autónoma de México; University of Illinois at Urbana-Champaign; University of Toronto; Space Telescope Science Institute; Yale University; New Mexico State University; University of Texas at Austin; Ohio State University; National Science Foundation; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution","keywords":"Quasar; Reverberation mapping; Acceleration; Physics; Astrophysics; Reverberation; Black hole (networking); Line (geometry); Absorption (acoustics); Optics; Computer science; Acoustics; Galaxy; Geometry; Classical mechanics","score_opus":0.017930811361804112,"score_gpt":0.2515074998291199,"score_spread":0.2335766884673158,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399527845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955959,0.000023175737,0.0015793835,0.000024539017,0.0000045087586,0.000020787598,0.0014086132,0.00021293078,0.0011302],"genre_scores_gemma":[0.9847077,0.000024795367,0.0067941966,0.000027211743,0.000013228345,0.000039482486,0.0073709525,0.00012245115,0.00089993206],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997515,0.000051195122,0.000009662675,0.000058152924,0.000088712375,0.00004081876],"domain_scores_gemma":[0.9993709,0.00008640654,0.00019401594,0.000109345245,0.00011204606,0.00012722942],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007762563,0.0003708086,0.00021879126,0.0014168824,0.00022586147,0.00026068604,0.00034165315,0.00021851358,0.0015342839],"category_scores_gemma":[0.0007939814,0.00014291536,0.0002405816,0.00074846216,0.00014804161,0.0002461,0.00048820022,0.00018780657,0.00052003324],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008247122,0.00070730137,0.74706495,0.00007561767,0.00023068674,0.00081450224,0.000769663,0.005851656,0.16474524,0.0005279676,0.005720886,0.0726669],"study_design_scores_gemma":[0.0000288875,0.00017586317,0.97985166,0.0000031726968,0.000025954616,0.00016104257,0.00008243374,0.004852458,0.012595301,0.00009317985,0.0021145677,0.0000154928],"about_ca_topic_score_codex":0.0038393582,"about_ca_topic_score_gemma":0.0048226905,"teacher_disagreement_score":0.0038393582,"about_ca_system_score_codex":0.00019652526,"about_ca_system_score_gemma":0.00014970273,"threshold_uncertainty_score":0.007633984},"labels":[],"label_agreement":null},{"id":"W4399597953","doi":"10.3847/1538-4357/ad7255","title":"Exploring Waveform Variations among Neutron Star Ray-tracing Codes for Complex Emission Geometries","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Nuclear Safety and Security Commission; European Research Council; Natural Sciences and Engineering Research Council of Canada; Centre National d’Etudes Spatiales; National Aeronautics and Space Administration","keywords":"Physics; Neutron star; Ray tracing (physics); RADIUS; Waveform; Pulsar; Astrophysics; Millisecond pulsar; Tracing; Observer (physics); Computational physics; Optics","score_opus":0.06413753714795645,"score_gpt":0.3404673296118831,"score_spread":0.27632979246392664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399597953","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97218835,0.000026551239,0.02578156,0.000060887254,0.000009756549,0.000018874985,0.00020752537,0.0007072492,0.0009992907],"genre_scores_gemma":[0.985827,0.000012276157,0.013538829,0.000008077217,0.0000028805698,0.000012533633,0.00031935124,0.00010396748,0.00017497787],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999551,0.000115840165,0.00004544572,0.00008701018,0.00015593009,0.00004476872],"domain_scores_gemma":[0.9933443,0.0042499797,0.000505854,0.0007855721,0.00094257056,0.00017164364],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001535616,0.0002460207,0.00019183602,0.00061582425,0.0002984577,0.0006165231,0.0006562881,0.00029646346,0.0007561806],"category_scores_gemma":[0.011590542,0.00013676716,0.00017566867,0.00052096124,0.00038320923,0.0006161729,0.0005762692,0.0004394354,0.0001146055],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091986294,0.00018541266,0.11663694,0.00011305224,0.0000937287,0.000347563,0.0011081145,0.7289784,0.036809783,0.012012632,0.0014646151,0.1013299],"study_design_scores_gemma":[0.000011589344,0.0000602654,0.0039940956,0.000004723467,0.0000055945,0.00003217344,0.000058195383,0.98473376,0.009841074,0.0009029067,0.00034581,0.00000982137],"about_ca_topic_score_codex":0.0025390282,"about_ca_topic_score_gemma":0.0020081725,"teacher_disagreement_score":0.0025390282,"about_ca_system_score_codex":0.00044627133,"about_ca_system_score_gemma":0.0004383879,"threshold_uncertainty_score":0.008121192},"labels":[],"label_agreement":null},{"id":"W4399629491","doi":"10.3847/1538-4357/ad402d","title":"Microgalaxies in LCDM","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"HORIZON EUROPE European Research Council; National Science Foundation","keywords":"Physics; Astrophysics; Dwarf galaxy; Velocity dispersion; Astronomy; Dark matter; Dark matter halo; Galaxy; Globular cluster; Cold dark matter; Dwarf galaxy problem; Population; Milky Way; Dwarf spheroidal galaxy; Halo; Interacting galaxy","score_opus":0.006437268430145028,"score_gpt":0.21654783150392434,"score_spread":0.21011056307377932,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399629491","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.992069,0.00019370783,0.00029752826,0.00015040845,0.000003497418,0.0000065023837,0.00018496516,0.000020592255,0.007073774],"genre_scores_gemma":[0.9988452,0.000040830633,0.000105436695,0.000016943151,0.0000020985635,0.0000014890172,0.00008739126,0.0000019297781,0.00089866226],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99987686,0.000020988517,0.0000053303434,0.000035226396,0.000019078865,0.00004244854],"domain_scores_gemma":[0.9995819,0.00007289699,0.00014921019,0.000055981363,0.000035623987,0.0001044522],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019892729,0.00008892467,0.00009355292,0.0007158953,0.00070597016,0.0008949489,0.00024041421,0.00021746353,0.008598557],"category_scores_gemma":[0.00087171525,0.00006775106,0.00008714045,0.0009183568,0.0006748021,0.00033577593,0.00093309063,0.00028718275,0.00047770992],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000091000395,0.000051869705,0.95931345,0.000023683922,0.000015509884,0.00062722166,0.00076910685,0.0015167125,0.0006879439,0.013968912,0.0010746714,0.021860048],"study_design_scores_gemma":[0.0000114595405,0.000040030965,0.97374445,0.000035046804,0.000015291756,0.0010223694,0.0018810995,0.0049085245,0.0006926133,0.00738522,0.010256267,0.0000076379965],"about_ca_topic_score_codex":0.020460606,"about_ca_topic_score_gemma":0.019931322,"teacher_disagreement_score":0.020460606,"about_ca_system_score_codex":0.0010010336,"about_ca_system_score_gemma":0.00035451172,"threshold_uncertainty_score":0.04068303},"labels":[],"label_agreement":null},{"id":"W4399675142","doi":"10.3847/1538-4357/ad34cf","title":"CLASSY. IX. The Chemical Evolution of the Ne, S, Cl, and Ar Elements","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Fundação para a Ciência e a Tecnologia; Office of Science; Agencia Nacional de Investigación y Desarrollo; Leibniz-Institut für Astrophysik Potsdam; Space Telescope Science Institute; European Southern Observatory; Istituto Nazionale di Astrofisica; York University; University of Minnesota; National Science Foundation; UK Research and Innovation; Arizona Board of Regents; Carnegie Mellon University; Leibniz-Gemeinschaft; University of Notre Dame; University of Arizona; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; National Aeronautics and Space Administration; U.S. Department of Energy","keywords":"Metallicity; Galaxy; Neon; Star formation; Galaxy formation and evolution; Abundance (ecology); Astrophysics; COSMIC cancer database; Physics; Redshift; Chemistry; Atomic physics; Ecology; Argon; Biology","score_opus":0.005261168592190174,"score_gpt":0.20768899453951548,"score_spread":0.2024278259473253,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399675142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98952323,0.00014295816,0.0002245505,0.000049723756,0.000006189133,0.000013024729,0.005271787,0.00003443735,0.0047340477],"genre_scores_gemma":[0.9918902,0.000064729305,0.0004740837,0.000043117117,0.00001293326,0.000014545375,0.004960344,0.000024299152,0.0025157551],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989307,0.000004185279,0.0000039786246,0.000036197525,0.000024225346,0.000038417733],"domain_scores_gemma":[0.99936205,0.00003553642,0.00031248754,0.00006384507,0.0000849151,0.00014109789],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001427526,0.00018936553,0.00015719446,0.0009696281,0.00034564413,0.00060588366,0.00021510934,0.00018479355,0.005079191],"category_scores_gemma":[0.000402571,0.00006413317,0.00019791756,0.0006172127,0.00018818083,0.0003481053,0.0004391171,0.00023962515,0.001259576],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012328224,0.000019114743,0.9802438,0.000019881723,0.000024165096,0.000038087146,0.00007291065,0.00014623566,0.0081042545,0.00028531245,0.00088105473,0.010041859],"study_design_scores_gemma":[0.000002171316,0.000016631944,0.9980234,0.0000018545913,0.0000024049455,0.000032927765,0.000035918558,0.0001433932,0.00057291536,0.000043469703,0.0011239337,9.658818e-7],"about_ca_topic_score_codex":0.00963479,"about_ca_topic_score_gemma":0.012004731,"teacher_disagreement_score":0.00963479,"about_ca_system_score_codex":0.0004355085,"about_ca_system_score_gemma":0.0001485212,"threshold_uncertainty_score":0.01915741},"labels":[],"label_agreement":null},{"id":"W4399741250","doi":"10.3847/1538-4357/ad4968","title":"Magnetic Fields Observed along the East–West Outflow of IRAS 16293-2422","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Protostar; Outflow; Astrophysics; Physics; Magnetic field; Wavelength; Millimeter; Polarization (electrochemistry); Submillimeter Array; Star formation; Stars; Optics; Chemistry","score_opus":0.02068854091031723,"score_gpt":0.23729406851147758,"score_spread":0.21660552760116036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399741250","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99722517,0.000028888991,0.000105596286,0.000018465358,0.0000053625445,0.000003833805,0.0004345371,0.000046085515,0.0021320654],"genre_scores_gemma":[0.9987816,0.000014133981,0.0001533538,0.000017000499,0.000006182203,0.0000030646563,0.0006578167,0.0000069615185,0.00035984378],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999442,0.0000032577543,0.0000023803073,0.000018478871,0.000013303032,0.000018311723],"domain_scores_gemma":[0.9998192,0.000010110582,0.0000536683,0.000014359457,0.0000297024,0.00007297274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007862158,0.00017458877,0.00019801834,0.0005280615,0.00032067712,0.00029443201,0.0001654135,0.00020917588,0.0014046109],"category_scores_gemma":[0.0001770253,0.00011039253,0.00009125308,0.0003720114,0.00014679099,0.00011809688,0.00031292206,0.0002542531,0.00033945174],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004208643,0.00020206496,0.6645766,0.00005276601,0.000099982855,0.0014069588,0.00047839395,0.0012287159,0.30499202,0.00029796467,0.0029416136,0.023302026],"study_design_scores_gemma":[0.0000074627796,0.000029209967,0.997329,0.0000027620872,0.0000048810098,0.000089690235,0.000053190815,0.00034946756,0.0015508061,0.00001867629,0.0005621983,0.0000026624414],"about_ca_topic_score_codex":0.0056214863,"about_ca_topic_score_gemma":0.010538424,"teacher_disagreement_score":0.0056214863,"about_ca_system_score_codex":0.00025735682,"about_ca_system_score_gemma":0.00013032863,"threshold_uncertainty_score":0.01117754},"labels":[],"label_agreement":null},{"id":"W4399911144","doi":"10.3847/1538-4357/ad571f","title":"Magnetic Fields in M-dwarf Members of the Pleiades Open Cluster Using APOGEE Spectra","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; U.S. Department of Energy; Smithsonian Institution; Vetenskapsrådet; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Ministério da Ciência, Tecnologia e Inovação; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Royal Swedish Academy of Sciences; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; Vanderbilt University; Swedish National Space Agency; New Mexico State University; University of Portsmouth; Yale University","keywords":"Physics; Astrophysics; Pleiades; Starspot; RADIUS; Stars; Open cluster; Magnetic field; Spectral line; Stellar rotation; Luminosity; Zeeman effect; Stellar classification; Astronomy; Galaxy","score_opus":0.017809257856749867,"score_gpt":0.25994486573660874,"score_spread":0.24213560787985888,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399911144","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99966025,0.00001355376,0.00006624246,0.0000024126557,2.6067917e-7,0.0000011235835,0.00014689483,0.0000052303762,0.00010405729],"genre_scores_gemma":[0.99923086,0.000011579583,0.00015038917,0.0000016905096,0.0000013784174,0.0000019175395,0.000517973,0.0000023724156,0.00008178194],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987817,0.00002523039,0.000007222564,0.0000537174,0.000021055022,0.0000145391705],"domain_scores_gemma":[0.9994295,0.00015810954,0.00015928138,0.000071829156,0.000063678504,0.00011757729],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037333302,0.00019655637,0.0001897923,0.00089326303,0.00024553636,0.00041057408,0.00016919056,0.00015677308,0.0007253983],"category_scores_gemma":[0.00094173045,0.00009687714,0.00019981065,0.0004025844,0.0002141365,0.0002160425,0.00049812003,0.00011359689,0.0002366206],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012512882,0.000015822086,0.99344057,0.000008641994,0.000035420922,0.000041789655,0.00032127544,0.0013848913,0.0016791075,0.000044466662,0.000088922585,0.0028139828],"study_design_scores_gemma":[0.0000022925417,0.00002943445,0.9981108,0.0000014942316,0.0000064693204,0.000048099682,0.0000954384,0.0013416433,0.00016553808,0.00002504596,0.00017092204,0.0000028435934],"about_ca_topic_score_codex":0.0057418044,"about_ca_topic_score_gemma":0.0067321183,"teacher_disagreement_score":0.0057418044,"about_ca_system_score_codex":0.000233223,"about_ca_system_score_gemma":0.00010165455,"threshold_uncertainty_score":0.011416793},"labels":[],"label_agreement":null},{"id":"W4399972766","doi":"10.3847/1538-4357/ad4a61","title":"Massive Interacting Binaries as an Enrichment Source for Multiple Populations in Star Clusters","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Ejecta; Stars; Population; Abundance (ecology); Binary star; Astronomy; Abundance of the chemical elements; Binary number; Stellar evolution; Supernova","score_opus":0.024406061370274557,"score_gpt":0.28790108423631217,"score_spread":0.2634950228660376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4399972766","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9963559,0.00006625214,0.002121127,0.000080081874,0.000005702569,0.0000066131092,0.00006800896,0.000051217517,0.00124513],"genre_scores_gemma":[0.99899226,0.000022681748,0.00036286577,0.000008405295,0.0000022644108,0.000002818844,0.00003828029,0.000009033092,0.0005613653],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998944,0.000022548258,0.000003361057,0.000024217248,0.000030708354,0.000024708224],"domain_scores_gemma":[0.99959284,0.00010993507,0.00007952046,0.000043047778,0.000039359893,0.00013534423],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039669147,0.00039976073,0.00051478116,0.0005447148,0.0008539448,0.0012967342,0.0008169611,0.00052229327,0.0022301949],"category_scores_gemma":[0.000822154,0.00017709873,0.0004089937,0.00041192758,0.00050645246,0.00057616376,0.0008792715,0.00032291823,0.00023214635],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004641666,0.00024212367,0.3077054,0.000060135797,0.00022016552,0.0010367908,0.00042313745,0.6379326,0.011255239,0.029054204,0.0015089612,0.010097106],"study_design_scores_gemma":[0.00006120356,0.00013990141,0.056750175,0.000013747478,0.000088437664,0.0002730775,0.00027142774,0.9301492,0.0024067217,0.00855953,0.0012484555,0.000038140126],"about_ca_topic_score_codex":0.011376899,"about_ca_topic_score_gemma":0.010299679,"teacher_disagreement_score":0.011376899,"about_ca_system_score_codex":0.0012683589,"about_ca_system_score_gemma":0.0005092082,"threshold_uncertainty_score":0.022621334},"labels":[],"label_agreement":null},{"id":"W4400070089","doi":"10.3847/1538-4357/ad43ea","title":"Systematically Revisiting All NuSTAR Spins of Black Holes in X-Ray Binaries","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":34,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Astrophysics; Spins; Physics; Black hole (networking); Astronomy; Computer science; Condensed matter physics","score_opus":0.01688888806654713,"score_gpt":0.2541889963224709,"score_spread":0.23730010825592376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400070089","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976866,0.00027153958,0.0007118949,0.000034751996,0.000008250215,0.0000081141225,0.0004711436,0.00002373877,0.00078399386],"genre_scores_gemma":[0.9981452,0.000097987686,0.00076689234,0.000020423175,0.000011922154,0.0000054189773,0.0007859979,0.000014418229,0.00015174907],"study_design_codex":"observational","study_design_gemma":"meta_analysis","domain_scores_codex":[0.9994067,0.00012640322,0.000090487025,0.00013935698,0.00015577486,0.00008119803],"domain_scores_gemma":[0.9951964,0.0014197256,0.001768874,0.00061085634,0.0006913989,0.00031273707],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017164905,0.00030450936,0.00042068586,0.004596016,0.0008113215,0.0017444362,0.0004063532,0.00025034734,0.0010181948],"category_scores_gemma":[0.008023561,0.00018063273,0.0002475355,0.0021195041,0.0006741256,0.00094734726,0.0019076677,0.00034098787,0.0003095752],"study_design_candidate":"meta_analysis","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009602705,0.000016783875,0.9823531,0.000043339947,0.000059906914,0.00008079505,0.0009267727,0.00021196716,0.0025041162,0.00027388424,0.0002541014,0.013179163],"study_design_scores_gemma":[0.0000031148136,0.00003445712,0.99338174,0.000032445096,0.000033718712,0.00018223557,0.0010630478,0.0011578265,0.0018959191,0.00060567376,0.0015987103,0.000011125234],"about_ca_topic_score_codex":0.0032350637,"about_ca_topic_score_gemma":0.008363467,"teacher_disagreement_score":0.004596016,"about_ca_system_score_codex":0.00029187664,"about_ca_system_score_gemma":0.0003110894,"threshold_uncertainty_score":0.009077787},"labels":[],"label_agreement":null},{"id":"W4400231542","doi":"10.3847/1538-4357/ad429c","title":"The Next Generation Deep Extragalactic Exploratory Public Near-infrared Slitless Survey Epoch 1 (NGDEEP-NISS1): Extragalactic Star-formation and Active Galactic Nuclei at 0.5 &lt; z &lt; 3.6","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"National Aeronautics and Space Administration; Science and Technology Facilities Council; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Active galactic nucleus; Galaxy; Redshift; Astronomy; Star formation; Photometry (optics); Spectral energy distribution; Supermassive black hole; Luminous infrared galaxy; Metallicity; Galaxy formation and evolution; Stars","score_opus":0.032390456547056065,"score_gpt":0.2352772228306202,"score_spread":0.2028867662835641,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400231542","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9058114,0.0001179939,0.0040316735,0.00021889391,0.000017147811,0.00014562315,0.081663154,0.00071578764,0.007278405],"genre_scores_gemma":[0.80485296,0.00011939139,0.018697489,0.00014790554,0.00002749207,0.00021325918,0.17104542,0.00015402595,0.004742015],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99965763,0.000060688406,0.000013781668,0.00009000405,0.00011834274,0.000059498976],"domain_scores_gemma":[0.9987342,0.0001240098,0.0002954619,0.00036787213,0.00020395576,0.00027450456],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00086470257,0.00033188873,0.0002790217,0.0011446931,0.00029293515,0.0004287719,0.0007348235,0.00028280602,0.002141984],"category_scores_gemma":[0.00091711467,0.00019766466,0.00030368366,0.0010243073,0.0001502887,0.0005009555,0.0012500886,0.00032573598,0.0008089711],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006085621,0.00032177614,0.9001882,0.00011957145,0.00017039222,0.000290209,0.0003105234,0.0036881233,0.01992914,0.0011047593,0.019550914,0.05371774],"study_design_scores_gemma":[0.000026580079,0.000042900752,0.98961395,0.000008467905,0.000014965319,0.000062879924,0.000045649806,0.0021371285,0.0023342906,0.00014531087,0.0055604284,0.0000074154173],"about_ca_topic_score_codex":0.0094091045,"about_ca_topic_score_gemma":0.024273155,"teacher_disagreement_score":0.0094091045,"about_ca_system_score_codex":0.00041031154,"about_ca_system_score_gemma":0.0003815208,"threshold_uncertainty_score":0.018708646},"labels":[],"label_agreement":null},{"id":"W4400272333","doi":"10.3847/1538-4357/ad45fa","title":"The FENIKS Survey: Multiwavelength Photometric Catalog in the UDS Field, and Catalogs of Photometric Redshifts and Stellar Population Properties","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; University of Toronto","funders":"Lawrence Berkeley National Laboratory; National Astronomical Observatories, Chinese Academy of Sciences; Japan Society for the Promotion of Science; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Universidad Nacional Autónoma de México; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ministério da Ciência, Tecnologia e Inovação; Cabinet Office, Government of Japan; Toray Science Foundation; High Energy Accelerator Research Organization; Ohio State University; Japan Science and Technology Agency; U.S. Department of Energy; Smithsonian Institution; National Aeronautics and Space Administration; Ministry of Education, Culture, Sports, Science and Technology; Academia Sinica; National Astronomical Observatory of Japan; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Physics; Redshift; Galaxy; Astrophysics; Photometry (optics); Photometric redshift; Algorithm; Stars; Computer science","score_opus":0.013913122887663694,"score_gpt":0.22988165581037645,"score_spread":0.21596853292271276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400272333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5651454,0.0016809067,0.010002968,0.00026361784,0.00007996243,0.00037484252,0.38856134,0.0026587083,0.031232337],"genre_scores_gemma":[0.43614185,0.0009555212,0.01960723,0.0001798273,0.00006284996,0.0005657182,0.5210118,0.00044704517,0.021028137],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992605,0.00009887456,0.000100712634,0.00017427275,0.00021504835,0.00015066954],"domain_scores_gemma":[0.9981674,0.00011184871,0.00039991623,0.00053572946,0.00049845054,0.00028660806],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010966,0.00030693642,0.00038681217,0.0059321155,0.0004024764,0.00073537376,0.00071545196,0.00019700274,0.01151573],"category_scores_gemma":[0.0026762902,0.00031774954,0.00023514523,0.005205075,0.00024107621,0.00094232004,0.0014623188,0.00019119983,0.0057761185],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049834186,0.000074548836,0.69591427,0.0004173679,0.0000654658,0.00015147228,0.0009132565,0.0013120834,0.0056374106,0.0038079277,0.11705228,0.17415564],"study_design_scores_gemma":[0.000026503902,0.000025015806,0.8838108,0.00008752049,0.000015465208,0.00013842162,0.00029707135,0.0008382859,0.0011023975,0.00058510905,0.11305251,0.000020812895],"about_ca_topic_score_codex":0.044031847,"about_ca_topic_score_gemma":0.046010163,"teacher_disagreement_score":0.044031847,"about_ca_system_score_codex":0.0009227954,"about_ca_system_score_gemma":0.0010478721,"threshold_uncertainty_score":0.08755112},"labels":[],"label_agreement":null},{"id":"W4400360045","doi":"10.3847/1538-4357/ad47f0","title":"The Green Bank 820 MHz Pulsar Survey. I. Survey Overview and Initial Results","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; McGill University","funders":"Precursory Research for Embryonic Science and Technology; Office of Naval Research; Alliance de recherche numérique du Canada; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Pulsar; Astrophysics; Green Bank Telescope; Galaxy; Astronomy; Millisecond pulsar","score_opus":0.04497683157123164,"score_gpt":0.37105119683431786,"score_spread":0.3260743652630862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400360045","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5542744,0.007573806,0.0047660647,0.002028514,0.0001927881,0.0014238268,0.38934293,0.0012341046,0.039163478],"genre_scores_gemma":[0.4858624,0.008093208,0.020725193,0.002690511,0.0005167447,0.0027309214,0.43866706,0.0005751272,0.040138796],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99931216,0.000112817244,0.0000448138,0.0001619975,0.00022512798,0.0001430729],"domain_scores_gemma":[0.9976428,0.00016586286,0.00036205677,0.0002345262,0.0008909726,0.0007037078],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013413758,0.000574431,0.0003793994,0.0044440106,0.0005356289,0.0007978855,0.0007850429,0.00039058801,0.00546467],"category_scores_gemma":[0.0010644586,0.00039771816,0.00022598813,0.0042109885,0.00023407178,0.00059792347,0.0012750116,0.00033067373,0.0062930523],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045911488,0.00014263316,0.8039362,0.0004260307,0.000098006494,0.00034117154,0.0005822077,0.000488536,0.0074092583,0.0004781065,0.09291141,0.09272728],"study_design_scores_gemma":[0.000022199201,0.00006433864,0.9460246,0.00007242264,0.000024451654,0.00014230236,0.00018713054,0.00026997417,0.00056233356,0.000047252684,0.052567206,0.000015838024],"about_ca_topic_score_codex":0.0898662,"about_ca_topic_score_gemma":0.14026552,"teacher_disagreement_score":0.0898662,"about_ca_system_score_codex":0.0011551435,"about_ca_system_score_gemma":0.0016268619,"threshold_uncertainty_score":0.1786862},"labels":[],"label_agreement":null},{"id":"W4400415119","doi":"10.3847/1538-4357/ad487e","title":"Chandra Study of the Proper Motion of HST-1 in the Jet of M87","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Nuclear Safety and Security Commission; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Knot (papermaking); Brightness; Proper motion; Superluminal motion; Radio galaxy; Flux (metallurgy); Offset (computer science); Very Long Baseline Array; Jet (fluid); Flare; Observable; Galaxy; Astronomy; Active galactic nucleus; Stars","score_opus":0.01134586521461016,"score_gpt":0.2328975352228706,"score_spread":0.22155167000826043,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400415119","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994492,0.00006206341,0.000060824295,0.00001174883,0.0000010936851,0.000001917238,0.00010670314,0.000007154694,0.00029929634],"genre_scores_gemma":[0.999335,0.000039316466,0.00016703784,0.000007887657,0.000005141091,0.000002100021,0.00036117152,0.0000060075417,0.000076418124],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985373,0.000019463549,0.000008493253,0.000027207037,0.000040064322,0.000051116585],"domain_scores_gemma":[0.99907434,0.00021320187,0.00030077554,0.00009865696,0.00011983311,0.00019319722],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036304924,0.00022417856,0.0003467131,0.0016325457,0.0004076693,0.00068675826,0.00036117388,0.00019798211,0.00050347374],"category_scores_gemma":[0.0010346052,0.00017242452,0.00028102566,0.0012926882,0.0002685773,0.00033038887,0.0005065968,0.00029853027,0.00019303584],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005636348,0.00025337693,0.93625927,0.00005873449,0.00015869629,0.0013546308,0.000886344,0.0039184047,0.03890797,0.0010569023,0.00082723645,0.015754791],"study_design_scores_gemma":[0.0000057838297,0.00003129128,0.99681646,0.0000058182686,0.0000113508195,0.000114471855,0.000072638286,0.0019538158,0.0007082738,0.000039693514,0.00023608921,0.0000042726383],"about_ca_topic_score_codex":0.0077409567,"about_ca_topic_score_gemma":0.011619821,"teacher_disagreement_score":0.0077409567,"about_ca_system_score_codex":0.00045548257,"about_ca_system_score_gemma":0.00021870159,"threshold_uncertainty_score":0.015391767},"labels":[],"label_agreement":null},{"id":"W4400415147","doi":"10.3847/1538-4357/ad4455","title":"Consistent Eccentricities for Gravitational-wave Astronomy: Resolving Discrepancies between Astrophysical Simulations and Waveform Models","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Department of Atomic Energy, Government of India; National Science Foundation","keywords":"Physics; Eccentricity (behavior); Gravitational wave; Globular cluster; Monte Carlo method; Binary number; Astrophysics; Statistical physics; Stars; Statistics","score_opus":0.03615885431224298,"score_gpt":0.3214591527687167,"score_spread":0.28530029845647376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400415147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9361383,0.000113372356,0.0586886,0.00027120364,0.000023384555,0.000030909974,0.0002878189,0.00019942549,0.0042468845],"genre_scores_gemma":[0.9918899,0.000044461278,0.0076301787,0.00002396489,0.000008192038,0.000019017094,0.00014869905,0.000052691827,0.00018308952],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9995863,0.00017838318,0.00003191081,0.00007597281,0.000091182235,0.000036224643],"domain_scores_gemma":[0.99397004,0.0039653354,0.0006893776,0.0007639401,0.00044184126,0.00016943815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0026343162,0.00024543828,0.00035722172,0.00064121344,0.00036510866,0.0010925921,0.0010106595,0.0005451823,0.0007734571],"category_scores_gemma":[0.017768778,0.00026278495,0.0002441334,0.00059801724,0.0005320404,0.0009768207,0.00061415375,0.00055238383,0.00014982326],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008892451,0.000049855837,0.031099604,0.000035829762,0.000039221213,0.00008985774,0.00015994557,0.9432598,0.0018107578,0.018457552,0.00032221578,0.00458652],"study_design_scores_gemma":[0.00001630998,0.000018013567,0.003120239,0.000009833517,0.0000064202286,0.000022055872,0.000024713327,0.99157834,0.0009078759,0.003999907,0.0002873038,0.000008951794],"about_ca_topic_score_codex":0.00671573,"about_ca_topic_score_gemma":0.004047931,"teacher_disagreement_score":0.00671573,"about_ca_system_score_codex":0.00081520004,"about_ca_system_score_gemma":0.00070565403,"threshold_uncertainty_score":0.013931751},"labels":[],"label_agreement":null},{"id":"W4400415600","doi":"10.3847/1538-4357/ad5310","title":"Time Delay of Fast Radio Burst Population with Respect to the Star Formation History","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Fundamental Research Funds for the Central Universities; National Natural Science Foundation of China","keywords":"Star (game theory); Astrophysics; Astronomy; Population; Physics; Demography; Sociology","score_opus":0.009174121188043508,"score_gpt":0.21231550969095303,"score_spread":0.20314138850290953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400415600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868367,0.00017777835,0.010324141,0.00007248287,0.0000040570562,0.000013064056,0.0010086069,0.00007029221,0.0014929634],"genre_scores_gemma":[0.99756575,0.000048056732,0.0008293025,0.000008081903,0.0000027039428,0.0000059094923,0.0010820734,0.00001262459,0.00044550328],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997303,0.000039374274,0.000008336723,0.000084633284,0.00007831496,0.00005907071],"domain_scores_gemma":[0.9985654,0.00054029305,0.0003495911,0.0001074061,0.00027660048,0.00016063385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00093380344,0.00016343321,0.00020046213,0.0009831332,0.00022422195,0.0006157385,0.0004414128,0.00029184963,0.0021041878],"category_scores_gemma":[0.0042495136,0.00015596882,0.00022330263,0.0006638548,0.00030933856,0.00037773082,0.00027539567,0.00025586612,0.00019708277],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023481577,0.000028551143,0.9317161,0.000034311004,0.00011171147,0.00010722103,0.00026554646,0.029134922,0.0074269585,0.005755116,0.00088414043,0.024300605],"study_design_scores_gemma":[0.000008590757,0.000025130365,0.9139248,0.000008527228,0.000036020385,0.00011993427,0.00010789141,0.08081789,0.0014712563,0.002299713,0.0011563665,0.000023809383],"about_ca_topic_score_codex":0.100050196,"about_ca_topic_score_gemma":0.051084958,"teacher_disagreement_score":0.100050196,"about_ca_system_score_codex":0.0012572249,"about_ca_system_score_gemma":0.00065950584,"threshold_uncertainty_score":0.19893569},"labels":[],"label_agreement":null},{"id":"W4400454153","doi":"10.3847/1538-4357/ad4d54","title":"The Long-period Spectroscopic Orbit and Dust Creation in the Wolf–Rayet Binary System WR 125","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Embry-Riddle Aeronautical University; Arizona Space Grant Consortium; Universities Space Research Association; Research Corporation for Science Advancement","keywords":"Physics; Photometry (optics); Astrophysics; Wolf–Rayet star; Orbital period; Astronomy; Stars","score_opus":0.007271457617245765,"score_gpt":0.24404192793881957,"score_spread":0.2367704703215738,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400454153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993387,0.000032784847,0.000041823187,0.000007110386,0.0000014200523,0.0000021610222,0.000060382394,0.0000033210033,0.00051230507],"genre_scores_gemma":[0.9997032,0.0000066819493,0.000048220227,0.0000031439188,0.0000014947884,0.0000010590039,0.00011102098,0.0000010786782,0.00012408753],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999491,0.000004751238,0.000004509313,0.000015115151,0.000013479357,0.000013054776],"domain_scores_gemma":[0.99982315,0.0000132829,0.000080888094,0.000012788339,0.000012567881,0.00005731161],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010957867,0.00012667794,0.00011243215,0.00050986384,0.00034030929,0.00036442728,0.00012557235,0.00017012299,0.0008904312],"category_scores_gemma":[0.00031424736,0.00007621919,0.000079296755,0.00025186187,0.00019195002,0.00015355142,0.0003443921,0.00017156238,0.0001892751],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004924616,0.00018910244,0.9277248,0.000021868373,0.000036540503,0.0010941265,0.00029736062,0.00045187326,0.06037886,0.00036552828,0.0003852513,0.008562243],"study_design_scores_gemma":[0.000007773061,0.000058171227,0.9978017,0.000002164029,0.0000050694916,0.00025532124,0.00007723674,0.00053738005,0.00086812326,0.00006423934,0.00031909344,0.0000036873425],"about_ca_topic_score_codex":0.0046842317,"about_ca_topic_score_gemma":0.0071900394,"teacher_disagreement_score":0.0046842317,"about_ca_system_score_codex":0.00025411107,"about_ca_system_score_gemma":0.000078400204,"threshold_uncertainty_score":0.009313941},"labels":[],"label_agreement":null},{"id":"W4400495272","doi":"10.3847/1538-4357/ad464b","title":"Updating the First CHIME/FRB Catalog of Fast Radio Bursts with Baseband Data","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":51,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Simon Fraser University; Banting Research Foundation; Canadian Institute for Theoretical Astrophysics; Perimeter Institute; University of Toronto; McGill University; York University; Fonds de Recherche du Québec – Nature et Technologies; University of British Columbia","funders":"Fonds de recherche du Québec – Nature et technologies; Canadian Space Agency; Smithsonian Astrophysical Observatory; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; National Research Council Canada; University of Toronto; Space Telescope Science Institute; McGill University; Alliance de recherche numérique du Canada; Industry Canada; Canarie; McGill Space Institute; Canadian Foundation for AIDS Research; Canadian Institute for Advanced Research; Canada Research Chairs; National Aeronautics and Space Administration; Government of Canada; National Science Foundation","keywords":"Physics; Baseband; Telescope; Radio telescope; Population; Polarization (electrochemistry); Astrophysics; Remote sensing","score_opus":0.015167421898873636,"score_gpt":0.30324718027861053,"score_spread":0.28807975837973687,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400495272","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.33878475,0.0068510827,0.02680608,0.0031708372,0.0017791408,0.00067094335,0.5621661,0.012916723,0.046854276],"genre_scores_gemma":[0.25293612,0.0021469474,0.051689614,0.0016388724,0.00076893065,0.00043902337,0.67431426,0.0031097846,0.012956469],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9970282,0.00014828298,0.00012502003,0.00038524804,0.0018912356,0.00042206977],"domain_scores_gemma":[0.978994,0.0012831531,0.001497407,0.005787031,0.010462582,0.001975798],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0039837114,0.00071863254,0.0008461125,0.008753494,0.0011353911,0.0026418704,0.0015507828,0.0006901234,0.0063060406],"category_scores_gemma":[0.011069592,0.000458411,0.0007095376,0.008036608,0.00043029798,0.001157434,0.00244551,0.0011410976,0.004584206],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008471014,0.00017148619,0.26809096,0.0006253769,0.0004931429,0.00057383545,0.0007790438,0.0043246956,0.022988671,0.0041785296,0.4101485,0.28677878],"study_design_scores_gemma":[0.00010284345,0.000057787074,0.48942485,0.00017662866,0.00014394257,0.0003232698,0.0001616591,0.0030891548,0.0075384662,0.00077128474,0.4980618,0.00014830104],"about_ca_topic_score_codex":0.2555668,"about_ca_topic_score_gemma":0.2844056,"teacher_disagreement_score":0.2555668,"about_ca_system_score_codex":0.00327174,"about_ca_system_score_gemma":0.004651102,"threshold_uncertainty_score":0.50815845},"labels":[],"label_agreement":null},{"id":"W4400495292","doi":"10.3847/1538-4357/ad4888","title":"Chronicling the Reionization History at 6 ≲ z ≲ 7 with Emergent Quasar Damping Wings","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":49,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Quasar; Physics; Redshift; Reionization; Astrophysics; Spectral line; Astronomy; Galaxy","score_opus":0.009929440652185243,"score_gpt":0.20845852494127293,"score_spread":0.1985290842890877,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400495292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993425,0.000010795038,0.0003357517,0.000030095282,8.975679e-7,0.000001415404,0.000089238376,0.000030248013,0.00015905807],"genre_scores_gemma":[0.99945587,0.000007899256,0.0003100328,0.0000049428227,0.0000010679415,0.000001301413,0.00015143417,0.000007418641,0.000060080307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992657,0.000014212136,0.0000035550916,0.000016331587,0.000017078946,0.000022211507],"domain_scores_gemma":[0.99927515,0.00023739944,0.00020448488,0.000062449355,0.000092352806,0.00012816512],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040438917,0.00023848146,0.0002017253,0.00056419993,0.00017909934,0.0005403885,0.00029764074,0.0002999104,0.0010035392],"category_scores_gemma":[0.0014013161,0.00019943646,0.0002499998,0.00037502078,0.00033796544,0.0005656225,0.0005189889,0.0003273227,0.000117497395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047705654,0.00020527655,0.6543057,0.000054421926,0.00019978736,0.00066066516,0.0005003812,0.28476694,0.040143643,0.0015555044,0.001244972,0.015885709],"study_design_scores_gemma":[0.000021621192,0.000105642284,0.422461,0.000009288097,0.00003875917,0.00010044442,0.0002929799,0.56342345,0.011948695,0.0010892825,0.00048037403,0.000028406701],"about_ca_topic_score_codex":0.0074606044,"about_ca_topic_score_gemma":0.0073912255,"teacher_disagreement_score":0.0074606044,"about_ca_system_score_codex":0.00043039047,"about_ca_system_score_gemma":0.00014260989,"threshold_uncertainty_score":0.014834344},"labels":[],"label_agreement":null},{"id":"W4400516971","doi":"10.3847/1538-4357/ad7500","title":"The First Catalog of Candidate White Dwarf–Main-sequence Binaries in Open Star Clusters: A New Window into Common Envelope Evolution","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Deutsches Elektronen-Synchrotron; Science Mission Directorate; Stockholms Universitet; Ministry of Education, India; University of Toronto; Agencia Nacional de Investigación y Desarrollo; Canada Research Chairs; California Institute of Technology; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Space Telescope Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Science Foundation","keywords":"White dwarf; Common envelope; Window (computing); Open cluster; White (mutation); Star (game theory); Sequence (biology); Envelope (radar); Biology; Physics; Astronomy; Astrophysics; Genetics; Computer science; Stars; Telecommunications","score_opus":0.016774550728575123,"score_gpt":0.25913843729829045,"score_spread":0.24236388656971533,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400516971","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976132,0.00025968027,0.0004874615,0.00001357343,0.0000025434713,0.000010003181,0.00067466835,0.000038682778,0.0009002529],"genre_scores_gemma":[0.9954892,0.00012045303,0.0011339459,0.000013129688,0.000007975985,0.000008145157,0.0028117804,0.000015589734,0.00039977656],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999777,0.000011474523,0.000016456428,0.00007648183,0.000063795116,0.000054796314],"domain_scores_gemma":[0.9990804,0.00015728938,0.0001984314,0.00013441016,0.000110571644,0.00031892152],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027366113,0.00020010617,0.00035578338,0.003411686,0.0009455587,0.0010367177,0.0004242259,0.0002265689,0.002216611],"category_scores_gemma":[0.00083922,0.00013553449,0.00019118669,0.0024914558,0.0003485619,0.00047651993,0.0011686427,0.00015193375,0.0005926614],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001903978,0.000071919916,0.96147954,0.00008877809,0.0000456709,0.00034535606,0.00033495392,0.0007455882,0.009850761,0.00073336007,0.0010809528,0.025032781],"study_design_scores_gemma":[0.0000075140865,0.000055965316,0.9932535,0.000017548757,0.00002547788,0.0003212183,0.0002747159,0.0019364066,0.0011970238,0.00029357304,0.0026080168,0.000009081932],"about_ca_topic_score_codex":0.005342207,"about_ca_topic_score_gemma":0.016027087,"teacher_disagreement_score":0.005342207,"about_ca_system_score_codex":0.00027136435,"about_ca_system_score_gemma":0.00048574188,"threshold_uncertainty_score":0.010622263},"labels":[],"label_agreement":null},{"id":"W4400587680","doi":"10.3847/1538-4357/ad463d","title":"Earliest Galaxies in the JADES Origins Field: Luminosity Function and Cosmic Star Formation Rate Density 300 Myr after the Big Bang","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":123,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; Ministerio de Ciencia e Innovación; Isaac Newton Trust; University of California, Santa Cruz; Johns Hopkins University; Danmarks Grundforskningsfond; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Science and Technology Facilities Council; National Research Foundation; UK Research and Innovation; Space Telescope Science Institute","keywords":"Physics; Redshift; Astrophysics; Galaxy; Luminosity function; Hubble Ultra-Deep Field; Astronomy; Photometry (optics); Star formation; Luminosity; Cosmic variance; James Webb Space Telescope; Hubble Deep Field; Advanced Camera for Surveys; Galaxy formation and evolution; Stars","score_opus":0.007977473051032092,"score_gpt":0.20438364354614494,"score_spread":0.19640617049511286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400587680","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99896336,0.00006375931,0.000083768646,0.000013897211,9.447652e-7,0.0000013404433,0.00038237587,0.000008120889,0.0004824552],"genre_scores_gemma":[0.99882656,0.000039020975,0.0001392377,0.0000067948818,0.0000046169444,0.0000017654686,0.0007116077,0.0000034307047,0.0002669126],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990904,0.000010185237,0.000005124029,0.000032045868,0.000017854096,0.000025760286],"domain_scores_gemma":[0.9990803,0.00013983806,0.0003298205,0.000086882086,0.00014223807,0.00022097176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003029558,0.00020003425,0.00016237386,0.0014805151,0.00028210424,0.000654657,0.00018170946,0.00014147932,0.0009971709],"category_scores_gemma":[0.0008671816,0.00011556683,0.00022204788,0.00048663633,0.00026554556,0.00033468165,0.0002817935,0.00017283899,0.00030239596],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005628597,0.000016863276,0.99270016,0.0000069999437,0.000028978591,0.000049229835,0.000107619555,0.0003043763,0.0033934815,0.00017734297,0.00016832196,0.00299053],"study_design_scores_gemma":[8.9707316e-7,0.0000074243594,0.9993643,0.0000016755826,0.0000037158402,0.00002746873,0.000025739451,0.00021610777,0.00018678914,0.000016502194,0.00014800734,0.000001322824],"about_ca_topic_score_codex":0.010191444,"about_ca_topic_score_gemma":0.013018805,"teacher_disagreement_score":0.010191444,"about_ca_system_score_codex":0.0004234724,"about_ca_system_score_gemma":0.00012919067,"threshold_uncertainty_score":0.020264268},"labels":[],"label_agreement":null},{"id":"W4400593758","doi":"10.3847/1538-4357/ad3dfb","title":"Decay Timescales of Chromospheric Condensations in Solar Flare Footpoints","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"University of Colorado Boulder; Goddard Space Flight Center; Queen's University; National Aeronautics and Space Administration; Queen's University Belfast; Ames Research Center; National Science Foundation","keywords":"Physics; Flare; Astrophysics; Solar flare; Spectrograph; Kinetic energy; Spectral line; Astronomy","score_opus":0.0063005428183754274,"score_gpt":0.23325546975963452,"score_spread":0.2269549269412591,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400593758","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985374,0.00015839955,0.0004484278,0.00000948561,0.0000017971612,0.0000036663137,0.00029931313,0.000020205594,0.00052127714],"genre_scores_gemma":[0.99958616,0.00002349455,0.000052968007,0.0000013920319,0.000001467277,0.0000018061693,0.00023149556,0.0000022704248,0.00009907766],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993885,0.0000036244796,0.0000032073403,0.00002159469,0.000014414429,0.0000182691],"domain_scores_gemma":[0.9993911,0.00017291556,0.00021568651,0.000042576103,0.000094999734,0.00008281323],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021938578,0.00010963993,0.00012190692,0.001024157,0.00017156107,0.0004263003,0.00013788401,0.00013905237,0.0015759126],"category_scores_gemma":[0.0016932631,0.00008557501,0.00011694888,0.00043934237,0.0001658954,0.0003977009,0.0002758224,0.00017131049,0.00020291244],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035550984,0.00003497664,0.94322824,0.000042077776,0.000060110375,0.0001452562,0.0005334285,0.0021768615,0.029380921,0.0009403123,0.00038591295,0.022716422],"study_design_scores_gemma":[0.0000029130506,0.000046143803,0.9927988,0.0000048535962,0.000008288053,0.00006997112,0.00013432743,0.0038291188,0.0024327221,0.00027389496,0.00039074314,0.000008171745],"about_ca_topic_score_codex":0.0034050583,"about_ca_topic_score_gemma":0.0020990316,"teacher_disagreement_score":0.0034050583,"about_ca_system_score_codex":0.00033302692,"about_ca_system_score_gemma":0.00006490513,"threshold_uncertainty_score":0.0067704916},"labels":[],"label_agreement":null},{"id":"W4400655378","doi":"10.3847/1538-4357/ad49a5","title":"Bursting with Feedback: The Relationship between Feedback Model and Bursty Star Formation Histories in Dwarf Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University; Perimeter Institute","funders":"Ministry of Colleges and Universities; Institut Périmètre de physique théorique; National Science Foundation; Government of Canada; University of Oklahoma; National Aeronautics and Space Administration","keywords":"Bursting; Dwarf galaxy; Star formation; Astrophysics; Galaxy; Star (game theory); Astronomy; Physics; Psychology; Neuroscience","score_opus":0.019791066400462277,"score_gpt":0.22862877164906134,"score_spread":0.20883770524859907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400655378","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996234,0.00001963736,0.0002252458,0.000010049813,6.59046e-7,8.979872e-7,0.000025915608,0.000010535237,0.000083508654],"genre_scores_gemma":[0.9998599,0.000006444277,0.00006287264,0.0000021427386,4.936837e-7,5.02436e-7,0.000031092237,0.0000023934476,0.00003416951],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989605,0.000032665215,0.000007903075,0.000028719822,0.000015823698,0.000018840703],"domain_scores_gemma":[0.99806803,0.0011372716,0.0003076858,0.00014970374,0.00011515167,0.00022215483],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047817783,0.00024987065,0.0001985534,0.00024835768,0.00016286277,0.0005385605,0.00037943214,0.0003213039,0.0008769609],"category_scores_gemma":[0.0032469789,0.0001756809,0.00027264495,0.00015388693,0.00027201764,0.00037452183,0.00034222868,0.00026593855,0.00006520893],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000247664,0.00010032942,0.7387409,0.000030001504,0.00014952947,0.00013119135,0.00011122127,0.24384704,0.011907044,0.00075181253,0.00013743414,0.0038457229],"study_design_scores_gemma":[0.000033030075,0.00017700739,0.3082945,0.000008034089,0.000051476774,0.000086135224,0.000087129774,0.68679684,0.0036776343,0.0006148523,0.0001591734,0.000014181531],"about_ca_topic_score_codex":0.008717374,"about_ca_topic_score_gemma":0.006185611,"teacher_disagreement_score":0.008717374,"about_ca_system_score_codex":0.00047768286,"about_ca_system_score_gemma":0.00014726176,"threshold_uncertainty_score":0.01733327},"labels":[],"label_agreement":null},{"id":"W4400655898","doi":"10.3847/1538-4357/ad4997","title":"Cloud Dissipation and Disk Wind in the Late Phase of Star Formation","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Astrophysics; Angular momentum; Outflow; Accretion (finance); Magnetohydrodynamics; Thermal wind; Protostar; Thick disk; Astronomy; Star formation; Magnetic field; Galaxy; Wind speed; Classical mechanics","score_opus":0.01366207423849136,"score_gpt":0.2769549597057389,"score_spread":0.26329288546724755,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400655898","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951652,0.00006115244,0.0016905782,0.00021218589,0.000020882762,0.000020156973,0.00022804072,0.00007262586,0.0025291673],"genre_scores_gemma":[0.99843127,0.000025565841,0.0009341226,0.00004370808,0.0000061449605,0.000015693531,0.00018014263,0.000018178307,0.00034502667],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998591,0.000033607666,0.0000067960445,0.00002147693,0.000023374298,0.000055644425],"domain_scores_gemma":[0.99920005,0.00037024345,0.000082722894,0.000044330853,0.00008151515,0.00022124076],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040245245,0.0004290565,0.00058452453,0.00030239797,0.00089474523,0.0010796979,0.0010507521,0.0012374541,0.0017547098],"category_scores_gemma":[0.0018462129,0.00031207447,0.0005728965,0.00039287156,0.0010565283,0.00064247113,0.0006914447,0.0010538528,0.0001648135],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021966272,0.00016031986,0.014848021,0.000019583887,0.000047844525,0.0002542304,0.000064140135,0.9801065,0.001811275,0.0012682785,0.0002461272,0.00095397205],"study_design_scores_gemma":[0.00009948702,0.000095278556,0.004922556,0.0000041537646,0.000013598658,0.000023867186,0.000052653355,0.99365294,0.0005219204,0.00039343679,0.00020872186,0.000011420845],"about_ca_topic_score_codex":0.028015068,"about_ca_topic_score_gemma":0.01314533,"teacher_disagreement_score":0.028015068,"about_ca_system_score_codex":0.0013245689,"about_ca_system_score_gemma":0.00099892,"threshold_uncertainty_score":0.055703998},"labels":[],"label_agreement":null},{"id":"W4400743920","doi":"10.3847/1538-4357/ad4f89","title":"Atmospheric Waves Driving Variability and Cloud Modulation on a Planetary-mass Object","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Brown dwarf; Photometry (optics); Light curve; Rossby wave; Effective temperature; Rotation period; Infrared; Astronomy; RADIUS; Planet; Stars; Atmospheric sciences","score_opus":0.005468057742304652,"score_gpt":0.2037839917580507,"score_spread":0.19831593401574604,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400743920","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99930024,0.000011545751,0.0002080822,0.0000062119916,0.0000010005081,0.0000023431485,0.000120385,0.000018294697,0.000332041],"genre_scores_gemma":[0.9996934,0.000004497523,0.00012662736,0.0000022473544,0.0000010148658,0.0000012045417,0.00013126226,0.000003669592,0.000036073176],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995196,0.0000053607773,0.0000030136719,0.000017347133,0.000010557521,0.000011751567],"domain_scores_gemma":[0.9997985,0.00005023946,0.000058784863,0.000023260054,0.000025974414,0.00004334879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018099944,0.0001914105,0.00012613962,0.00043784082,0.00024619832,0.00035560824,0.00020056251,0.0002083657,0.00079723995],"category_scores_gemma":[0.0005316528,0.00015396383,0.00034348413,0.0003257146,0.00017378922,0.00019049176,0.00022377772,0.00015607399,0.0001385213],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014091663,0.000047696787,0.93198067,0.000024878505,0.000057585614,0.00015882123,0.00011701353,0.009435979,0.052008513,0.00027401026,0.00031869535,0.0054351888],"study_design_scores_gemma":[0.000005873309,0.000019133888,0.9826592,0.0000018498168,0.000011600907,0.000038262937,0.000038601822,0.015798246,0.001262698,0.00005689337,0.0001041208,0.0000034123523],"about_ca_topic_score_codex":0.009496871,"about_ca_topic_score_gemma":0.00875474,"teacher_disagreement_score":0.009496871,"about_ca_system_score_codex":0.00043014786,"about_ca_system_score_gemma":0.00014894226,"threshold_uncertainty_score":0.018883169},"labels":[],"label_agreement":null},{"id":"W4400743935","doi":"10.3847/1538-4357/ad4ed6","title":"A Hot Core in the Group-dominant Elliptical Galaxy NGC 777","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics","score_opus":0.011627385336076148,"score_gpt":0.23304827504178924,"score_spread":0.22142088970571308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400743935","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99914,0.00004266905,0.000111081565,0.000007407263,8.5483526e-7,0.0000014023423,0.00003746767,0.000018713721,0.00064037926],"genre_scores_gemma":[0.99971086,0.000009019131,0.00011371393,0.0000030004833,0.000001258444,9.718021e-7,0.00004485255,0.0000046518244,0.000111513764],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999536,0.0000045093334,0.0000015233443,0.000009942332,0.000011393495,0.000018958697],"domain_scores_gemma":[0.9997981,0.00003337025,0.00005446195,0.000030819636,0.000027701128,0.000055624427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007753426,0.00013961291,0.0002066586,0.00048017406,0.00026138587,0.0004177299,0.00018716995,0.00016744585,0.00086043734],"category_scores_gemma":[0.00024074683,0.000101064,0.000121518824,0.00024229982,0.00033840406,0.0001609296,0.00039054372,0.00009057288,0.00024036427],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048936036,0.00007484221,0.5937063,0.000094798095,0.00012080436,0.002181369,0.0013382585,0.0033424427,0.3800758,0.0021641448,0.00097144465,0.015440276],"study_design_scores_gemma":[0.000016952243,0.000110119,0.97680795,0.0000107385695,0.00003929437,0.0005853981,0.00041942502,0.003761947,0.0160402,0.0005414161,0.0016519481,0.00001448801],"about_ca_topic_score_codex":0.0046629934,"about_ca_topic_score_gemma":0.0048604794,"teacher_disagreement_score":0.0046629934,"about_ca_system_score_codex":0.0004125597,"about_ca_system_score_gemma":0.00012156448,"threshold_uncertainty_score":0.009271681},"labels":[],"label_agreement":null},{"id":"W4400744561","doi":"10.3847/1538-4357/ad4796","title":"Are These Planets or Brown Dwarfs? Broadly Solar Compositions from High-resolution Atmospheric Retrievals of ∼10–30 M <sub>Jup</sub> Companions","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":45,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Astrophysics Division; Heising-Simons Foundation; National Science Foundation","keywords":"Brown dwarf; Planet; Physics; High resolution; Exoplanet; Astrobiology; Astrophysics; Environmental science; Astronomy; Atmospheric sciences; Remote sensing; Geology","score_opus":0.01357301941686371,"score_gpt":0.22497715032114415,"score_spread":0.21140413090428045,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400744561","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976349,0.00014843607,0.0011163526,0.000026578422,0.0000037172078,0.0000026851599,0.00041765126,0.00009042719,0.000559174],"genre_scores_gemma":[0.9983581,0.000038922146,0.00087676453,0.000011468666,0.0000049816927,0.0000010280717,0.0006022588,0.000014416752,0.00009209943],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999037,0.000008252603,0.0000075219605,0.00004500677,0.000016831938,0.000018701146],"domain_scores_gemma":[0.9997596,0.000058012363,0.000088602756,0.00003975183,0.000027189588,0.000026847947],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023689846,0.00017544153,0.00021710018,0.0004780436,0.00022800178,0.00041512834,0.00023038652,0.00023454626,0.000907762],"category_scores_gemma":[0.0006664133,0.0001678026,0.00024171238,0.000445796,0.00015783819,0.00048164075,0.00031286717,0.00014043832,0.00035733037],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018094311,0.000026398457,0.90529186,0.00006774013,0.00015097024,0.00021134307,0.0002932032,0.0018436644,0.06573457,0.00025971807,0.00056062115,0.025378942],"study_design_scores_gemma":[0.000009673905,0.000023437668,0.97673744,0.00000822011,0.000056655343,0.00027922395,0.00016158409,0.015500259,0.0055331187,0.00029010978,0.0013915757,0.000008736961],"about_ca_topic_score_codex":0.0034961249,"about_ca_topic_score_gemma":0.010837341,"teacher_disagreement_score":0.0034961249,"about_ca_system_score_codex":0.00019356482,"about_ca_system_score_gemma":0.00010065284,"threshold_uncertainty_score":0.006951511},"labels":[],"label_agreement":null},{"id":"W4400789353","doi":"10.3847/1538-4357/ad4e35","title":"Sensitive 3 mm Imaging of Discrete Sources in the Fields of Thermal Sunyaev–Zel’dovich Effect–Selected Galaxy Clusters","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Jet Propulsion Laboratory; National Research Foundation; California Institute of Technology; National Aeronautics and Space Administration; Agence Nationale de la Recherche; University of California, Los Angeles; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy cluster; Galaxy; Cluster (spacecraft); Sunyaev–Zel'dovich effect; Spectral index; Cluster sampling; South Pole Telescope; Telescope; Population; Astronomy; Spectral line","score_opus":0.003345723130279285,"score_gpt":0.20960902382574226,"score_spread":0.20626330069546298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400789353","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980039,0.00006789723,0.0011532895,0.000015074041,0.000002046318,0.000003395603,0.00016918349,0.000043722175,0.0005415599],"genre_scores_gemma":[0.9988482,0.000015209529,0.00084449945,0.000008540533,0.0000026128257,0.0000027059039,0.00015026508,0.0000055879673,0.00012243688],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998504,0.000022472042,0.0000053524577,0.000042038115,0.000029864974,0.000049821527],"domain_scores_gemma":[0.9995474,0.00012751124,0.00011735489,0.0000721854,0.00004025028,0.000095158044],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032741943,0.00012293842,0.00018072646,0.0007711392,0.00024059195,0.0003583912,0.00020034844,0.00017591541,0.0013964017],"category_scores_gemma":[0.00042943825,0.0002209181,0.00018312859,0.00033489676,0.00019393335,0.00015735086,0.00047720657,0.0001295489,0.00019303252],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001173457,0.0001040581,0.75956786,0.00007294555,0.0001727518,0.00046905948,0.00047171782,0.006326225,0.2111086,0.0006917859,0.0007166826,0.019124879],"study_design_scores_gemma":[0.000028485505,0.000087251305,0.9777884,0.0000056370623,0.00003082251,0.0002457974,0.00010415065,0.005984269,0.01498767,0.00018309959,0.00054075045,0.000013577645],"about_ca_topic_score_codex":0.0021503055,"about_ca_topic_score_gemma":0.004231013,"teacher_disagreement_score":0.0021503055,"about_ca_system_score_codex":0.0002839007,"about_ca_system_score_gemma":0.000117593,"threshold_uncertainty_score":0.004671395},"labels":[],"label_agreement":null},{"id":"W4400823521","doi":"10.3847/1538-4357/ad3de8","title":"The Early Ultraviolet Light Curves of Type II Supernovae and the Radii of Their Progenitor Stars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Agencia Estatal de Investigación; Stockholms Universitet; Deutsches Elektronen-Synchrotron; Liverpool John Moores University; Israel Science Foundation; Trinity College Dublin; Institut National de Physique Nucléaire et de Physique des Particules; Northwestern University; University of Warwick; Alexander Family Foundation; University of Leicester; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Weizmann Institute of Science; Minerva Foundation; California Institute of Technology; National Science Foundation; University of Washington; Gordon and Betty Moore Foundation","keywords":"Physics; Light curve; Astrophysics; Supernova; Stars; RADIUS; Astronomy","score_opus":0.007604725402602081,"score_gpt":0.2194322972225213,"score_spread":0.21182757181991924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400823521","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990158,0.000032860196,0.00013512297,0.0000034608572,5.450883e-7,0.0000014214372,0.00042998546,0.000011392498,0.0003692831],"genre_scores_gemma":[0.9980769,0.000034778954,0.00016379285,0.0000022338945,0.0000017353825,0.00000265949,0.0014643618,0.000007452411,0.00024602455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999007,0.000014793554,0.000009043929,0.000028478524,0.0000208372,0.000026147372],"domain_scores_gemma":[0.9989743,0.00029433897,0.00031608695,0.00009314811,0.000100835045,0.00022126547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032118688,0.00023542116,0.00015117737,0.001208803,0.00014323488,0.00051053014,0.00021529544,0.00019462116,0.0015020238],"category_scores_gemma":[0.0017131813,0.0001375195,0.00024533112,0.00042499966,0.00016000344,0.00029150897,0.00027268368,0.00018241635,0.0005059405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010771131,0.00002528063,0.9891739,0.000007131559,0.00003963358,0.000047266614,0.00006630405,0.0023452379,0.0043683746,0.00015280071,0.00018800133,0.0034784414],"study_design_scores_gemma":[0.0000031558736,0.000039383674,0.9958633,0.0000031399147,0.000008686731,0.0001512287,0.0000448643,0.002497977,0.0009621008,0.0001002717,0.00032152832,0.000004374232],"about_ca_topic_score_codex":0.002456352,"about_ca_topic_score_gemma":0.0028314455,"teacher_disagreement_score":0.002456352,"about_ca_system_score_codex":0.00022180835,"about_ca_system_score_gemma":0.00006126818,"threshold_uncertainty_score":0.0050247908},"labels":[],"label_agreement":null},{"id":"W4400834356","doi":"10.3847/1538-4357/ad4f8c","title":"Spectrum and Polarization of the Galactic Center Radio Transient ASKAP J173608.2–321635 from THOR-GC and VLITE","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Calgary","funders":"Office of Naval Research; Russian Academy of Sciences; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; Leibniz-Institut für Astrophysik Potsdam; Rheinische Friedrich-Wilhelms-Universität Bonn; Leibniz-Gemeinschaft; Jet Propulsion Laboratory; Universität Hamburg; Max-Planck-Gesellschaft; U.S. Naval Research Laboratory; Eberhard Karls Universität Tübingen; European Commission; California Institute of Technology; Associated Universities; National Science Foundation","keywords":"Physics; Polarization (electrochemistry); Analytical Chemistry (journal); Astrophysics; Chemistry","score_opus":0.004492909007192105,"score_gpt":0.1969102707701511,"score_spread":0.192417361762959,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400834356","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9954797,0.00009696458,0.0003199747,0.00007344995,0.000016853757,0.000009716623,0.0016483427,0.000112684975,0.0022423735],"genre_scores_gemma":[0.99395907,0.000041264215,0.00029403024,0.000037166297,0.00001477185,0.000010747929,0.0049687875,0.000030459852,0.0006436561],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984443,0.000012846086,0.000008764699,0.00004104456,0.0000489287,0.000043903136],"domain_scores_gemma":[0.99963963,0.000038156086,0.00006937784,0.00004694886,0.00008940846,0.00011651957],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000275176,0.0003202943,0.0003116279,0.0010032505,0.00049108156,0.0004923154,0.00033367935,0.00037281998,0.0016624967],"category_scores_gemma":[0.00036697907,0.00018717372,0.0002780527,0.00096012774,0.00021890707,0.00023525245,0.00051008846,0.00033785007,0.00070299226],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0017238494,0.00029730564,0.7314863,0.00018234325,0.00027636898,0.0045660394,0.0012398632,0.0029265855,0.21971884,0.0005789289,0.007239776,0.029763801],"study_design_scores_gemma":[0.000034793065,0.00006588795,0.98862773,0.000008719179,0.00004597089,0.00048692012,0.00021303928,0.0021884777,0.0051292577,0.000077544704,0.003101877,0.000019616975],"about_ca_topic_score_codex":0.005809184,"about_ca_topic_score_gemma":0.0065486236,"teacher_disagreement_score":0.005809184,"about_ca_system_score_codex":0.00041939857,"about_ca_system_score_gemma":0.00020206874,"threshold_uncertainty_score":0.0115507245},"labels":[],"label_agreement":null},{"id":"W4400893158","doi":"10.3847/1538-4357/ad5daf","title":"Erratum: “Bangs and Meteors from the Quiet Comet 15P/Finlay” (2015, ApJ, 814, 79)","year":2024,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":false,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Meteoroid; QUIET; Comet; Astronomy","score_opus":0.008849509902010697,"score_gpt":0.22580290429088803,"score_spread":0.21695339438887734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400893158","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.00037275974,0.0012229283,0.000116706695,0.05029496,0.9337482,0.000016026182,0.0021059602,0.00029086706,0.011831592],"genre_scores_gemma":[0.0129475305,0.0048697805,0.0012421795,0.11310898,0.33123404,0.00010212547,0.008077781,0.0014210542,0.52699655],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99851185,0.00011936633,0.00028526393,0.00025095398,0.00068246236,0.00015004136],"domain_scores_gemma":[0.99535334,0.00072612235,0.00043776244,0.00041173975,0.002569249,0.0005018172],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016297424,0.002555081,0.0014945271,0.003819462,0.0056812367,0.0045537157,0.0023883271,0.005010296,0.061179735],"category_scores_gemma":[0.012843563,0.0008634379,0.0013935314,0.001689433,0.0016209015,0.0029168024,0.0024232687,0.0060899407,0.046151813],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024481637,0.000004737363,0.000078321595,0.000026445021,0.000004211686,0.0001168182,0.000012915566,0.0000089296955,0.00003220765,0.00030662943,0.9978527,0.0015316391],"study_design_scores_gemma":[0.00003105835,0.0000244313,0.0028516327,0.00016018351,0.000025844445,0.00026008487,0.00013330892,0.00007012905,0.00021862735,0.0010370462,0.99516016,0.000027328351],"about_ca_topic_score_codex":0.042782977,"about_ca_topic_score_gemma":0.05323199,"teacher_disagreement_score":0.061179735,"about_ca_system_score_codex":0.0038276385,"about_ca_system_score_gemma":0.0039628255,"threshold_uncertainty_score":0.20466655},"labels":[],"label_agreement":null},{"id":"W4400936269","doi":"10.3847/1538-4357/ad4886","title":"SpectAcLE: An Improved Method for Modeling Light Echo Spectra","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Spectroscopy and Laser Applications","field":"Chemistry","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Division of Astronomical Sciences; Israel Science Foundation; National Aeronautics and Space Administration","keywords":"Physics; Echo (communications protocol); Spectral line; Spectacle; Astrophysics; Astronomy; Optics","score_opus":0.014069050239597177,"score_gpt":0.3122619846569713,"score_spread":0.2981929344173741,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400936269","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.004491667,0.000027318983,0.99370676,0.00004912781,0.000022941573,0.000020655503,0.00009472957,0.0011106232,0.0004761672],"genre_scores_gemma":[0.16090538,0.00012045557,0.83113295,0.00012298184,0.00008680874,0.00021154004,0.0004931798,0.0018766082,0.0050501046],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99952745,0.00015935655,0.000024100647,0.00007512525,0.00017024793,0.000043728705],"domain_scores_gemma":[0.99821055,0.00090308336,0.0001460364,0.00021235489,0.00044910965,0.0000789577],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017930553,0.0010131964,0.0005863293,0.0013567713,0.00065146066,0.0013585802,0.0024901894,0.0016885181,0.0051164567],"category_scores_gemma":[0.0057173455,0.0006857158,0.0014632897,0.00087544357,0.0005637202,0.001704212,0.00094153173,0.0017263357,0.0017592576],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014920755,0.00009337811,0.0024981727,0.00008255487,0.00010574701,0.00015894728,0.00013228855,0.8880292,0.0131187,0.017008087,0.0029784846,0.07564521],"study_design_scores_gemma":[0.0000028769068,0.0000035557869,0.000042867687,0.0000018159553,0.0000020407329,0.000010105218,0.0000028039376,0.9981516,0.000370193,0.0009194845,0.00048721206,0.00000540183],"about_ca_topic_score_codex":0.015252911,"about_ca_topic_score_gemma":0.01188805,"teacher_disagreement_score":0.015252911,"about_ca_system_score_codex":0.0007559832,"about_ca_system_score_gemma":0.0015750658,"threshold_uncertainty_score":0.030328274},"labels":[],"label_agreement":null},{"id":"W4400937784","doi":"10.3847/1538-4357/ad2b62","title":"Mapping the Milky Way in 5D with 170 Million Stars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Jet Propulsion Laboratory; California Institute of Technology; Eötvös Loránd Tudományegyetem; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; FAS Division of Science, Harvard University; Gordon and Betty Moore Foundation; Harvard University; University of California, Los Angeles","keywords":"Physics; Milky Way; Stars; Astronomy; Astrophysics; Stellar kinematics; Star count; K-type main-sequence star; T Tauri star","score_opus":0.015762073458816542,"score_gpt":0.21680177605081727,"score_spread":0.2010397025920007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400937784","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9224443,0.0013353694,0.0077642924,0.0003011163,0.000051507606,0.00004124068,0.056313667,0.002321227,0.009427306],"genre_scores_gemma":[0.8507452,0.00051724556,0.016981088,0.00016476637,0.00006141399,0.0000706986,0.12701342,0.00055055117,0.0038955486],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995809,0.000054346365,0.000021760916,0.00014973678,0.00012516907,0.00006812844],"domain_scores_gemma":[0.9994136,0.000065406755,0.00012692872,0.00013691286,0.00010978984,0.00014729958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065955054,0.00036589685,0.00034579722,0.0021709732,0.000347729,0.0010189784,0.0003818177,0.00028828497,0.0031408914],"category_scores_gemma":[0.0017046672,0.0002189883,0.0005266031,0.0021386489,0.00018651897,0.0006552678,0.0015643955,0.00027495544,0.0029652598],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041186696,0.00014925726,0.7859878,0.0003493763,0.00057081215,0.0005427847,0.002269351,0.008970815,0.009562801,0.0035446032,0.06383843,0.12380208],"study_design_scores_gemma":[0.000057029778,0.00007925166,0.77595943,0.00010879409,0.00011446628,0.00024890847,0.00085512653,0.010140097,0.0031741094,0.00215301,0.20707376,0.00003603611],"about_ca_topic_score_codex":0.016882055,"about_ca_topic_score_gemma":0.022333667,"teacher_disagreement_score":0.016882055,"about_ca_system_score_codex":0.00037986715,"about_ca_system_score_gemma":0.0004291571,"threshold_uncertainty_score":0.033567607},"labels":[],"label_agreement":null},{"id":"W4400979970","doi":"10.3847/1538-4357/ad5842","title":"Variable Radio Emission of Neutron Star X-Ray Binary Ser X–1 during Its Persistent Soft State","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge","funders":"","keywords":"Physics; Neutron star; Astrophysics; X-ray binary; Binary number; Variable star; Binary star; Astronomy; Star (game theory); Stars","score_opus":0.01074619753429806,"score_gpt":0.21879959137022895,"score_spread":0.20805339383593088,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400979970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995522,0.00006159294,0.00003338486,0.0000038701432,0.0000016748254,9.996102e-7,0.000041817882,0.0000026787202,0.00030183455],"genre_scores_gemma":[0.9996896,0.00002549953,0.00004710872,0.000004381384,0.0000042616916,0.0000010452173,0.00013613964,0.0000012402608,0.0000906716],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999285,0.000010795086,0.0000052832374,0.000023924104,0.000013874311,0.000017759396],"domain_scores_gemma":[0.9995982,0.00008084391,0.00018760524,0.000028161554,0.000037927108,0.000067332156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001754887,0.00013817409,0.00015717857,0.0006745263,0.00024813545,0.00041812233,0.00012967164,0.00016045797,0.00079857506],"category_scores_gemma":[0.00043053742,0.00008142446,0.000080941936,0.00025054865,0.00018017174,0.00015100103,0.0002656499,0.00016581539,0.00021054813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058464357,0.00009614268,0.92499566,0.000042443506,0.000044463784,0.00082271197,0.00025261805,0.00031211379,0.06537413,0.00015703341,0.00013560851,0.0071823667],"study_design_scores_gemma":[0.000004410671,0.00010570318,0.99673826,0.0000041703834,0.000011980464,0.0004455306,0.000066722,0.00033172424,0.00201557,0.000028225428,0.00024473577,0.0000028763588],"about_ca_topic_score_codex":0.0005405312,"about_ca_topic_score_gemma":0.00067920145,"teacher_disagreement_score":0.00079857506,"about_ca_system_score_codex":0.00010985394,"about_ca_system_score_gemma":0.00003824789,"threshold_uncertainty_score":0.0026715398},"labels":[],"label_agreement":null},{"id":"W4400998278","doi":"10.3847/1538-4357/ad5353","title":"The Mass Density of Merging Binary Black Holes over Cosmic Time","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; COSMIC cancer database; Binary number; Astrophysics; Binary black hole; Astronomy; Gravitational wave","score_opus":0.005102656143219141,"score_gpt":0.23717908397031712,"score_spread":0.23207642782709798,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400998278","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977018,0.0002022583,0.00042749985,0.00004239249,0.0000021558371,0.0000022505626,0.00021849928,0.000028181268,0.0013748725],"genre_scores_gemma":[0.9994468,0.000051051218,0.00008745039,0.0000050481117,0.00000471022,0.0000016016335,0.00021027171,0.0000037658083,0.00018920747],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998286,0.000030275485,0.000008990306,0.000050785864,0.000035891262,0.000045544868],"domain_scores_gemma":[0.9982529,0.0006383068,0.00067145674,0.00011512446,0.00013273675,0.00018948458],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049198273,0.00012104259,0.00014197272,0.0013769718,0.00022226204,0.0008788828,0.00033420595,0.0003860969,0.0027350998],"category_scores_gemma":[0.003508128,0.00013573094,0.00016822506,0.0007395071,0.0003142839,0.0007012844,0.00038622538,0.00015960405,0.00036046442],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019246538,0.000027815091,0.9727338,0.00002109981,0.00007292027,0.00016814239,0.00033169313,0.004611082,0.0038963596,0.0057555665,0.000495735,0.011693377],"study_design_scores_gemma":[0.000015259873,0.00008043694,0.9747493,0.000014028591,0.000051405754,0.0005129569,0.0003147123,0.017812254,0.0020356535,0.0028485951,0.0015486132,0.00001691671],"about_ca_topic_score_codex":0.0032580118,"about_ca_topic_score_gemma":0.0021969185,"teacher_disagreement_score":0.0032580118,"about_ca_system_score_codex":0.00048947043,"about_ca_system_score_gemma":0.0000988068,"threshold_uncertainty_score":0.009149849},"labels":[],"label_agreement":null},{"id":"W4400999003","doi":"10.3847/1538-4357/ad4da2","title":"First Detection of CO Isotopologues in a High-redshift Main-sequence Galaxy: Evidence of a Top-heavy Stellar Initial Mass Function","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Fundamental Research Funds for the Central Universities; Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China","keywords":"Physics; Isotopologue; Astrophysics; Galaxy; Redshift; Astronomy; Stellar mass; Initial mass function; Function (biology); Sequence (biology); Star formation; Spectral line","score_opus":0.022222346211785645,"score_gpt":0.26463923150449287,"score_spread":0.24241688529270722,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4400999003","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990778,0.000028620912,0.0003931246,0.00001286657,0.0000012716737,0.0000039200686,0.00006798377,0.00003282718,0.00038143352],"genre_scores_gemma":[0.9994836,0.000009709555,0.00031708766,0.000009808009,0.0000011996809,0.0000013542767,0.000085877014,0.000002737322,0.000088616565],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991095,0.000010017026,0.000003672008,0.000027823537,0.000024526802,0.000022926164],"domain_scores_gemma":[0.99944884,0.000096772834,0.00010382428,0.00008161495,0.00007935796,0.000189634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038755388,0.00024911587,0.00018559629,0.0005082517,0.0005345746,0.00039285643,0.00039490187,0.00045608715,0.0008208448],"category_scores_gemma":[0.00044751097,0.00024614413,0.00027696765,0.00024071262,0.00038973242,0.00021807151,0.0004489952,0.00030275105,0.0001961273],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019239869,0.00008617526,0.9293702,0.00002187678,0.00007605739,0.0002202431,0.00018431789,0.0012527832,0.06465404,0.00021194274,0.00018496237,0.0035450393],"study_design_scores_gemma":[0.000007995887,0.00015109811,0.98434305,0.0000028518346,0.000027731321,0.0001310924,0.00006168495,0.0070823636,0.007723537,0.00010069346,0.00036218218,0.000005590937],"about_ca_topic_score_codex":0.008212338,"about_ca_topic_score_gemma":0.018366024,"teacher_disagreement_score":0.008212338,"about_ca_system_score_codex":0.0007277351,"about_ca_system_score_gemma":0.00016532661,"threshold_uncertainty_score":0.01632905},"labels":[],"label_agreement":null},{"id":"W4401079728","doi":"10.3847/1538-4357/ad4f84","title":"Spectroscopic Survey of Faint Planetary-nebula Nuclei. V. The EGB 6-type Central Star of Abell 57*","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Planetary Science Division; Leibniz-Gemeinschaft; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; Jet Propulsion Laboratory; Leibniz-Institut für Astrophysik Potsdam; Eötvös Loránd Tudományegyetem; National Central University; Gordon and Betty Moore Foundation; Queen's University Belfast; Durham University; York University; Space Telescope Science Institute; Ohio State University; University of Texas at Austin; Carnegie Mellon University; Pennsylvania State University; Los Alamos National Laboratory; College of Engineering, Michigan State University; University of Washington; European Space Agency; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Queen's University; Harvard University; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; New Mexico State University; University of California, Los Angeles; University of Portsmouth; Vanderbilt University; Science Mission Directorate; Yale University; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Star (game theory); Planetary nebula; Emission nebula; Nebula; Stars","score_opus":0.014217043796503551,"score_gpt":0.2347404785944641,"score_spread":0.22052343479796055,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401079728","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982084,0.00012062906,0.00005008681,0.00003487761,0.0000052084197,0.00000396475,0.00046282943,0.0000105534755,0.0011034473],"genre_scores_gemma":[0.99703693,0.00009964322,0.00028994805,0.000050823997,0.000013524912,0.0000050248814,0.0016927622,0.000006965707,0.0008043419],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998778,0.0000065699733,0.0000069458956,0.0000360638,0.000035974423,0.000036678284],"domain_scores_gemma":[0.99964285,0.000016588225,0.0000757909,0.000021627036,0.00006523162,0.00017797627],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001963814,0.0002372875,0.00035133093,0.0010349172,0.00075394206,0.0003479339,0.00022934286,0.00023119521,0.0010042284],"category_scores_gemma":[0.00021655088,0.0001088964,0.00016602517,0.0004168353,0.0002264087,0.0001588395,0.0005065587,0.00026940004,0.0005396671],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014816607,0.00014524416,0.9300098,0.000035280336,0.000046691803,0.0012735744,0.00053198327,0.00006305543,0.059625108,0.00019436299,0.0010151371,0.0069117816],"study_design_scores_gemma":[0.0000031855575,0.000032553042,0.99710804,0.0000038063174,0.000006202219,0.0003515037,0.000102750055,0.00006373382,0.0011628829,0.000014484407,0.0011490841,0.0000018975903],"about_ca_topic_score_codex":0.016333975,"about_ca_topic_score_gemma":0.033002514,"teacher_disagreement_score":0.016333975,"about_ca_system_score_codex":0.00075651,"about_ca_system_score_gemma":0.00032624445,"threshold_uncertainty_score":0.032477796},"labels":[],"label_agreement":null},{"id":"W4401141022","doi":"10.3847/1538-4357/ad4ee2","title":"Filaments of the Slime Mold Cosmic Web and How They Affect Galaxy Evolution","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Slime Mold and Myxomycetes Research","field":"Engineering","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University","funders":"Division of Astronomical Sciences; Israel Science Foundation; National Energy Research Scientific Computing Center; United States - Israel Binational Science Foundation; Alfred P. Sloan Foundation","keywords":"Physics; Protein filament; Galaxy; Astrophysics; Materials science","score_opus":0.008508835492782998,"score_gpt":0.22563269480745868,"score_spread":0.21712385931467568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401141022","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9970962,0.000077012504,0.0018315159,0.00003686906,0.0000024875972,0.0000025474,0.000092476184,0.00005394145,0.0008069768],"genre_scores_gemma":[0.9991937,0.000025193434,0.0005962569,0.000006169726,0.0000019312433,0.0000016929669,0.000060008784,0.000010302169,0.00010475743],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999267,0.000019316805,0.0000031372767,0.000019724,0.000015613612,0.000015596317],"domain_scores_gemma":[0.99910814,0.00029272866,0.0003480312,0.000075240474,0.00006553872,0.00011032823],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019191597,0.00015799087,0.00017260348,0.00063533895,0.00028981996,0.0009276015,0.00022409778,0.00024062383,0.0010994682],"category_scores_gemma":[0.0024613778,0.00016634526,0.00021140791,0.0003471012,0.00040190533,0.00044472385,0.00032534802,0.0002665254,0.00011479033],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003331802,0.00006549795,0.77479887,0.00008102988,0.00020479251,0.00064246915,0.0006366866,0.14523298,0.03742495,0.010933673,0.0013050201,0.028340861],"study_design_scores_gemma":[0.0000241637,0.000109084656,0.6377871,0.000039059556,0.00008942238,0.000359775,0.00040006865,0.3386145,0.010825877,0.009107091,0.0026003548,0.000043473592],"about_ca_topic_score_codex":0.005541478,"about_ca_topic_score_gemma":0.004612253,"teacher_disagreement_score":0.005541478,"about_ca_system_score_codex":0.00044425137,"about_ca_system_score_gemma":0.00011603944,"threshold_uncertainty_score":0.011018455},"labels":[],"label_agreement":null},{"id":"W4401148821","doi":"10.3847/1538-4357/ad5afc","title":"Nuclear Uncertainties Associated with the Nucleosynthesis in Ejecta of a Black Hole Accretion Disk","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"TRIUMF","funders":"Los Alamos National Laboratory; Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; National Science Foundation","keywords":"Nucleosynthesis; Physics; Ejecta; Accretion (finance); Astrophysics; Isotope; Nuclear reaction; Stellar nucleosynthesis; Black hole (networking); Abundance of the chemical elements; Abundance (ecology); Neutron; Nuclear physics; Stars; Supernova","score_opus":0.011625280743523028,"score_gpt":0.25234969513494804,"score_spread":0.240724414391425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401148821","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953998,0.00012801432,0.0032944311,0.000044123728,0.000004716528,0.000004610628,0.00023230238,0.000046504185,0.00084560603],"genre_scores_gemma":[0.9989982,0.000026714375,0.00061414007,0.0000054041743,0.000002302015,0.000002769881,0.00021937594,0.000017604847,0.000113485265],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9995628,0.00014336847,0.00004032317,0.000107213586,0.00011342137,0.000032893364],"domain_scores_gemma":[0.9957833,0.0029867769,0.00042439427,0.00029859896,0.0003878395,0.00011909112],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022231275,0.0004457297,0.00038893273,0.0007677681,0.0005509828,0.0009553181,0.00067343627,0.0006361958,0.0009263045],"category_scores_gemma":[0.00862075,0.00035620082,0.0006100217,0.0006373518,0.0006693454,0.00078768656,0.0007318614,0.00043872197,0.00015012958],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036820295,0.00004764657,0.115794726,0.000042950403,0.00019188075,0.00028841107,0.00008475697,0.87115586,0.007078928,0.0015626627,0.00010150651,0.0032825395],"study_design_scores_gemma":[0.000038523696,0.00010573764,0.09018726,0.000023720568,0.000063762214,0.00014716285,0.00010448802,0.8954143,0.011552641,0.0019417014,0.00037506668,0.000045624194],"about_ca_topic_score_codex":0.009587286,"about_ca_topic_score_gemma":0.0053385394,"teacher_disagreement_score":0.009587286,"about_ca_system_score_codex":0.0013699555,"about_ca_system_score_gemma":0.00028088797,"threshold_uncertainty_score":0.019062996},"labels":[],"label_agreement":null},{"id":"W4401171270","doi":"10.3847/1538-4357/ad4a2a","title":"Final Moments. II. Observational Properties and Physical Modeling of Circumstellar-material-interacting Type II Supernovae","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":64,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Nuclear Safety and Security Commission; Natural Sciences and Engineering Research Council of Canada; European Commission; Canada Research Chairs; National Aeronautics and Space Administration; National Centre for Supercomputing Applications; University of California Berkeley; University of Illinois at Urbana-Champaign; University of Toronto; Villum Fonden; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Spectral line; Ejecta; Light curve; Brightness; Radiative transfer; Ultraviolet; Astronomy; Optics","score_opus":0.060999186060895084,"score_gpt":0.2649729614307193,"score_spread":0.20397377536982422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401171270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98496604,0.00005868428,0.008334489,0.00003088563,0.0000063965967,0.000015549002,0.00059116865,0.00010868672,0.005888136],"genre_scores_gemma":[0.99797446,0.000016780728,0.00087035476,0.0000022108595,0.0000043012583,0.000005423975,0.00048980437,0.00001094208,0.0006258205],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988604,0.000018812254,0.000008642433,0.000022965309,0.000030831256,0.000032606713],"domain_scores_gemma":[0.99945587,0.00009411985,0.00019171613,0.00007600253,0.00006964023,0.00011262598],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003152487,0.00020944291,0.00014490631,0.0005634991,0.00029074488,0.0008649374,0.00042685372,0.00014098885,0.0016116351],"category_scores_gemma":[0.0015197984,0.000103400256,0.00034593965,0.00030839248,0.00021102426,0.0003443719,0.00044668055,0.00019387198,0.0003157399],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00062507327,0.00012963527,0.79368204,0.00003780745,0.000105621846,0.0006641163,0.00020514654,0.15555473,0.008230271,0.022769185,0.0010685852,0.016927829],"study_design_scores_gemma":[0.000035120072,0.00023604442,0.5363708,0.000013464831,0.000049568014,0.0005927106,0.00029417203,0.44238958,0.006458455,0.009513929,0.004014095,0.000032032556],"about_ca_topic_score_codex":0.003844302,"about_ca_topic_score_gemma":0.0029839014,"teacher_disagreement_score":0.003844302,"about_ca_system_score_codex":0.00050899055,"about_ca_system_score_gemma":0.00019008372,"threshold_uncertainty_score":0.007643819},"labels":[],"label_agreement":null},{"id":"W4401193885","doi":"10.3847/1538-4357/ad3e83","title":"Search for Gravitational-lensing Signatures in the Full Third Observing Run of the LIGO–Virgo Network","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":69,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Polytechnique Montréal; Perimeter Institute; University of British Columbia","funders":"European Social Fund; Great Southern Development Commission, Government of Western Australia; Japan Society for the Promotion of Science; Science and Technology Facilities Council; National Science and Technology Council; ICTP South American Institute for Fundamental Research; Division of Human Resource Development; Ministry of Science and ICT, South Korea; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, India; National Research Foundation of Korea; Korea Astronomy and Space Science Institute; Hungarian Scientific Research Fund; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; Generalitat de Catalunya; U.S. Department of Energy; National Natural Science Foundation of China; Agencia Estatal de Investigación; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Govern de les Illes Balears; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministry of Education, Culture, Sports, Science and Technology; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Ministerio de Ciencia e Innovación; European Commission; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; Abdus Salam International Centre for Theoretical Physics; Institute for Cosmic Ray Research, University of Tokyo; Centre National de la Recherche Scientifique; Council of Scientific and Industrial Research, India; National Research Foundation; Fonds De La Recherche Scientifique - FNRS; Russian Foundation for Basic Research; Institut des Origines de Lyon; Russian Science Foundation; Leverhulme Trust; Scottish Funding Council; European Regional Development Fund; Scottish Universities Physics Alliance; Centres de Recerca de Catalunya; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; LIGO; Astrophysics; Gravitational lens; Strong gravitational lensing; Gravitational wave; Cosmology; Astronomy; Dark matter; Binary black hole; Sky; Redshift; Galaxy","score_opus":0.01996822902916491,"score_gpt":0.32400977403255615,"score_spread":0.30404154500339126,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401193885","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998268,0.00002434419,0.00064923626,0.000026793297,0.0000019671713,0.000007463333,0.0005584994,0.00005811671,0.00040540038],"genre_scores_gemma":[0.99703765,0.000010102415,0.0011763584,0.000010176329,0.0000042144234,0.000008143028,0.0016188115,0.000013247448,0.000121312085],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987174,0.00026031476,0.000052028507,0.00029554832,0.00037292103,0.00030184689],"domain_scores_gemma":[0.9949641,0.001114894,0.0014093393,0.00092648505,0.0004211635,0.0011640303],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020717077,0.0003101155,0.000495293,0.0021751598,0.0005533554,0.00088012055,0.00050531636,0.0004129093,0.000895039],"category_scores_gemma":[0.0045366352,0.00021531228,0.0007104997,0.0013591957,0.0003006353,0.00040141444,0.0016410891,0.00043131254,0.00022529472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00042061668,0.00007441479,0.9805038,0.000014128214,0.00028845386,0.00016796218,0.0001581251,0.0028014688,0.006417646,0.00023888316,0.0003112553,0.00860324],"study_design_scores_gemma":[0.000015403835,0.000086739055,0.9857737,0.0000073526803,0.00008739543,0.00014416315,0.000083450104,0.010945986,0.0019886196,0.00022152401,0.0006293551,0.000016259624],"about_ca_topic_score_codex":0.009907096,"about_ca_topic_score_gemma":0.017843623,"teacher_disagreement_score":0.009907096,"about_ca_system_score_codex":0.0005607466,"about_ca_system_score_gemma":0.00058862113,"threshold_uncertainty_score":0.019698858},"labels":[],"label_agreement":null},{"id":"W4401202866","doi":"10.3847/1538-4357/ad65d7","title":"Environments around Quasars at z ∼ 3 Revealed by Wide-field Imaging with Subaru HSC and CFHT","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Saint Mary's University; Herzberg Institute of Astrophysics","funders":"Planetary Science Division; National Astronomical Observatories, Chinese Academy of Sciences; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; Higher Education Discipline Innovation Project; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; National Central University; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; Centre National de la Recherche Scientifique; Chinese Academy of Sciences; Eötvös Loránd Tudományegyetem; Academia Sinica; Japan Science and Technology Agency; Smithsonian Institution; Canadian Foundation for AIDS Research; National Natural Science Foundation of China; Space Telescope Science Institute; National Science Foundation; Compute Canada; Los Alamos National Laboratory; Princeton University; Johns Hopkins University; Queen's University Belfast; National Aeronautics and Space Administration; Durham University","keywords":"Quasar; Physics; Astrophysics; Galaxy; Subaru Telescope; Sky; Halo; Astronomy; Local Group; Milky Way; Spectral line; Spectrograph","score_opus":0.0038111467231386046,"score_gpt":0.1935545716731891,"score_spread":0.1897434249500505,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401202866","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99908495,0.00003358485,0.0001440324,0.000013704853,5.42179e-7,0.0000013652548,0.00019362167,0.00001844515,0.00050976116],"genre_scores_gemma":[0.9995202,0.00001515658,0.00021211075,0.000006226771,0.000002772909,0.0000011198608,0.000186516,0.000002534579,0.00005337844],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992406,0.000007186891,0.0000030010892,0.000013006743,0.000017294222,0.000035468758],"domain_scores_gemma":[0.99961925,0.000049011775,0.00011781963,0.00003498227,0.000055366014,0.00012348863],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017346522,0.00009839058,0.000121049976,0.0016357391,0.00028236635,0.00039732616,0.0001174891,0.00015224046,0.0008929537],"category_scores_gemma":[0.00034497288,0.000099124656,0.00012349735,0.0008911234,0.00021110133,0.0002916413,0.00037997254,0.000119648306,0.00014852856],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008765441,0.000019062194,0.9620549,0.000008209353,0.000028652308,0.0002817945,0.00056431093,0.00026251635,0.025710559,0.00019450653,0.00046849143,0.010319383],"study_design_scores_gemma":[6.59945e-7,0.0000064101555,0.9989795,0.0000011774939,0.0000047038347,0.000062909254,0.00014050056,0.00024162726,0.00039838496,0.000026870091,0.000135418,0.0000018207093],"about_ca_topic_score_codex":0.012700578,"about_ca_topic_score_gemma":0.02579258,"teacher_disagreement_score":0.012700578,"about_ca_system_score_codex":0.00022138262,"about_ca_system_score_gemma":0.00010575036,"threshold_uncertainty_score":0.025253296},"labels":[],"label_agreement":null},{"id":"W4401219332","doi":"10.3847/1538-4357/ad499b","title":"Impact of Higher Harmonics of Gravitational Radiation on the Population Inference of Binary Black Holes","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Tata Institute of Fundamental Research; Department of Atomic Energy, Government of India; Canadian Institute for Advanced Research; California Institute of Technology; National Science Foundation","keywords":"Physics; Astrophysics; Binary number; Gravitational wave; Harmonics; Astronomy; Population; Binary black hole; Medicine; Quantum mechanics","score_opus":0.0143300181193678,"score_gpt":0.3033923441224489,"score_spread":0.2890623260030811,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401219332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97216845,0.000232547,0.024668645,0.00019469929,0.000018210041,0.00001190045,0.00021435657,0.00007463618,0.0024166477],"genre_scores_gemma":[0.99823016,0.000028008748,0.00149589,0.00002931065,0.000010715957,0.0000028796696,0.00010846871,0.00001046806,0.00008409346],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99641114,0.002094579,0.00014790657,0.0006982635,0.00043621252,0.00021196704],"domain_scores_gemma":[0.95723563,0.035597447,0.0026788877,0.0027713708,0.0010828238,0.0006338774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.008596085,0.0002903767,0.0004839563,0.00092050387,0.00057128194,0.0016898658,0.00068818755,0.0005766302,0.001697656],"category_scores_gemma":[0.045082305,0.00025425383,0.00042578674,0.0004255725,0.0007946906,0.0015328637,0.0011922444,0.00061795645,0.00024298136],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046969263,0.0000630555,0.9139251,0.00007444286,0.0003032153,0.000165362,0.00042651792,0.03102129,0.0062619178,0.008498789,0.0004729442,0.038317658],"study_design_scores_gemma":[0.000051020448,0.00019065522,0.5459865,0.00011592765,0.00035057485,0.0006300674,0.00068293186,0.40878618,0.02019647,0.020352507,0.0025792858,0.00007799815],"about_ca_topic_score_codex":0.0027219197,"about_ca_topic_score_gemma":0.002945804,"teacher_disagreement_score":0.008596085,"about_ca_system_score_codex":0.0004956441,"about_ca_system_score_gemma":0.00037811897,"threshold_uncertainty_score":0.04546094},"labels":[],"label_agreement":null},{"id":"W4401226490","doi":"10.3847/1538-4357/ad4ee0","title":"A Hot Mess: The Rich and Complex Soft Emitting Regions Surrounding the Reflection Dominated Flaring Central Engine of Mrk 1239","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Active galactic nucleus; Ionization; Torus; Plasma; Emission spectrum; Astronomy; Interstellar medium; Reflection (computer programming); Spectral line; Ion; Geometry","score_opus":0.02457717064443784,"score_gpt":0.26558063817646665,"score_spread":0.2410034675320288,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401226490","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9959927,0.00017205285,0.0005361468,0.00012425282,0.000010024203,0.0000067192345,0.00026329042,0.000091084505,0.0028038004],"genre_scores_gemma":[0.9985587,0.000032600627,0.0005695356,0.00004108986,0.000013799156,0.0000021578533,0.0002059203,0.00002757349,0.00054861885],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995244,0.0000025117586,0.0000019860213,0.00001611296,0.000009917065,0.000017044258],"domain_scores_gemma":[0.9998307,0.00001134463,0.00008137437,0.000014380508,0.000012017748,0.000050079587],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000073750816,0.00026365803,0.00024619623,0.0006128644,0.0006474785,0.00068485306,0.0003556876,0.0003337799,0.002572162],"category_scores_gemma":[0.00018393867,0.00016411471,0.00018108524,0.0003562382,0.0004052165,0.00038249296,0.00086234603,0.00036070158,0.0007239415],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011164581,0.00015402294,0.46218836,0.00023599528,0.0001779546,0.038762193,0.0025888907,0.001536169,0.44566652,0.0016236284,0.0037593239,0.04219034],"study_design_scores_gemma":[0.000009341851,0.00009599174,0.97969455,0.000016557367,0.00003309082,0.00851679,0.001201987,0.0007383504,0.005011416,0.00039167897,0.004266164,0.000024156854],"about_ca_topic_score_codex":0.0023257523,"about_ca_topic_score_gemma":0.0033071234,"teacher_disagreement_score":0.002572162,"about_ca_system_score_codex":0.00023443604,"about_ca_system_score_gemma":0.0000886545,"threshold_uncertainty_score":0.008604705},"labels":[],"label_agreement":null},{"id":"W4401226694","doi":"10.3847/1538-4357/ad5a09","title":"Repelling Planet Pairs by Ping-pong Scattering","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"RES’EAU-WaterNET; National Aeronautics and Space Administration","keywords":"Physics; Planet; Angular momentum; Astrophysics; Scattering; Astronomy; Classical mechanics; Quantum mechanics","score_opus":0.007089348851809774,"score_gpt":0.2061119643172598,"score_spread":0.19902261546545003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401226694","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97388047,0.000111841786,0.01988717,0.00016382255,0.000052473908,0.000025005542,0.00004550776,0.00013487053,0.0056987386],"genre_scores_gemma":[0.9982206,0.000021145945,0.0009392248,0.00003015611,0.000010998151,0.0000060839366,0.00003172403,0.000015502072,0.00072455395],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997576,0.000050425184,0.0000068699374,0.000056039495,0.000061548526,0.00006749052],"domain_scores_gemma":[0.9989273,0.0004938177,0.00016776891,0.00012797433,0.000084113286,0.00019906052],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00037418818,0.00026019165,0.00046001922,0.00048777252,0.00086686155,0.00054202165,0.0006691955,0.0006605054,0.0029619501],"category_scores_gemma":[0.0023467657,0.00030693438,0.00032820387,0.00025902313,0.00069056154,0.0006840289,0.001150592,0.0006231878,0.0004449908],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019243432,0.00048995763,0.12461588,0.0004980708,0.0005432696,0.013489969,0.0025312703,0.29917645,0.37258115,0.09205743,0.008635568,0.083456665],"study_design_scores_gemma":[0.000114468094,0.00057623506,0.045960557,0.000025958749,0.00007285339,0.0038360101,0.00068036997,0.8868403,0.021335736,0.036055557,0.0043958747,0.000106081054],"about_ca_topic_score_codex":0.0009542575,"about_ca_topic_score_gemma":0.00079313637,"teacher_disagreement_score":0.0029619501,"about_ca_system_score_codex":0.0002785016,"about_ca_system_score_gemma":0.00017304151,"threshold_uncertainty_score":0.009908736},"labels":[],"label_agreement":null},{"id":"W4401226846","doi":"10.3847/1538-4357/ad528c","title":"Direct Optimal Mapping Image Power Spectrum and its Window Functions","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; European Commission; Canadian Institute for Advanced Research; National Science Foundation; American Academy of Periodontology Foundation; Gordon and Betty Moore Foundation; FP7 International Cooperation; Science and Technology Facilities Council; National Research Foundation; UK Research and Innovation; Space Telescope Science Institute; Massachusetts Institute of Technology; National Aeronautics and Space Administration","keywords":"Reionization; Physics; Spectral density; Window function; Window (computing); Power (physics); Image (mathematics); Astrophysics; Computer science; Computer vision; Galaxy; Redshift","score_opus":0.007671040702659358,"score_gpt":0.21361062404318404,"score_spread":0.20593958334052467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401226846","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47816512,0.000103671424,0.51787275,0.00007917684,0.00001938359,0.00003061069,0.00010904949,0.00040060462,0.003219681],"genre_scores_gemma":[0.9416036,0.00005303874,0.05745597,0.000011798368,0.0000051656043,0.000023148381,0.000094349016,0.00006804089,0.00068497914],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99993134,0.000013264311,0.000003009546,0.000015654716,0.000025145038,0.000011608716],"domain_scores_gemma":[0.99976796,0.00011638637,0.000022239688,0.000033303746,0.00004667335,0.000013382013],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024997216,0.00032605228,0.00015128525,0.00028951038,0.0001067189,0.0003292277,0.00027904887,0.00020267443,0.0010262678],"category_scores_gemma":[0.0011522576,0.00015350794,0.00018328532,0.00019817721,0.00028172607,0.00057208404,0.00020346674,0.00020416362,0.000116380645],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032327257,0.00011164556,0.005675358,0.00010178715,0.000048911752,0.00040473405,0.00017378831,0.70688236,0.1694841,0.028755965,0.00083943666,0.08719866],"study_design_scores_gemma":[0.0000060991856,0.0000147734445,0.0014631075,0.0000018492968,0.000002386554,0.000045609075,0.000011256035,0.98475707,0.011462443,0.0020140267,0.00021494509,0.00000635181],"about_ca_topic_score_codex":0.00093646167,"about_ca_topic_score_gemma":0.00038485392,"teacher_disagreement_score":0.0010262678,"about_ca_system_score_codex":0.00024165129,"about_ca_system_score_gemma":0.00020786487,"threshold_uncertainty_score":0.0034332275},"labels":[],"label_agreement":null},{"id":"W4401343039","doi":"10.3847/1538-4357/ad54c2","title":"Neutron Star Atmosphere–Ocean Dynamics","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Perimeter Institute","funders":"HORIZON EUROPE European Research Council; Jet Propulsion Laboratory","keywords":"Physics; Neutron star; Magnetohydrodynamics; Magnetohydrodynamic drive; Plasmoid; Astrophysics; Plasma; Vortex; Mechanics; Nuclear physics; Magnetic reconnection","score_opus":0.004542773850295926,"score_gpt":0.21706073474701754,"score_spread":0.21251796089672162,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401343039","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9897719,0.00027685866,0.0036448217,0.00015500694,0.000016511745,0.000005159074,0.00031769558,0.00003989664,0.005772104],"genre_scores_gemma":[0.9983645,0.00015591859,0.00051593885,0.000015215552,0.000008291927,0.0000030764045,0.00022614606,0.000011061951,0.0006998083],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999454,0.000011976631,0.0000027315077,0.000016710346,0.000011967406,0.000011216816],"domain_scores_gemma":[0.9998951,0.000017285427,0.000030483994,0.000008915885,0.000022568429,0.000025687605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010017752,0.00019712881,0.00027215306,0.00033055272,0.00024390587,0.00052406185,0.00016894456,0.00029395014,0.0013186435],"category_scores_gemma":[0.0004292056,0.00011604763,0.00029931427,0.00026095135,0.00028295704,0.00041929501,0.0006078543,0.0002802083,0.00016665802],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003684866,0.00010224583,0.3022105,0.00015018517,0.0003543777,0.00087957096,0.00038028858,0.5589279,0.058633428,0.054445054,0.0019293983,0.021618593],"study_design_scores_gemma":[0.000043618806,0.00008051707,0.17578208,0.000021651478,0.00004067573,0.00015732157,0.00023188065,0.8088597,0.0032198045,0.007908148,0.00361738,0.00003724359],"about_ca_topic_score_codex":0.009106109,"about_ca_topic_score_gemma":0.0043159914,"teacher_disagreement_score":0.009106109,"about_ca_system_score_codex":0.0004269445,"about_ca_system_score_gemma":0.00024853772,"threshold_uncertainty_score":0.018106222},"labels":[],"label_agreement":null},{"id":"W4401345860","doi":"10.3847/1538-4357/ad5722","title":"Connections between Planetary Populations and Chemical Characteristics of Their Host Stars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of International Science and Engineering; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Lawrence Berkeley National Laboratory; Ministry of Science and ICT, South Korea; Universidad Nacional Autónoma de México; University of Oxford; York University; National Research Foundation of Korea; Joint Institute for Nuclear Astrophysics - Center for the Evolution of the Elements; Leibniz-Gemeinschaft; University of Notre Dame; Ohio State University; National Research Foundation; Carnegie Mellon University; University of Washington; European Space Agency; Alfred P. Sloan Foundation; Johns Hopkins University; University of Utah; Carnegie Institution of Washington; Smithsonian Institution; U.S. Department of Energy; California Institute of Technology; Ministério da Ciência, Tecnologia e Inovação; National Aeronautics and Space Administration; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; National Science Foundation","keywords":"Planet; Physics; Astrobiology; Stars; Astronomy; Exoplanet; Planetary system; Abundance (ecology); Astrophysics; Kepler-47; Planetary migration; Biology; Ecology","score_opus":0.019159159982812903,"score_gpt":0.2376539050459101,"score_spread":0.2184947450630972,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401345860","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992704,0.000067306355,0.0000630251,0.000004020278,7.768479e-7,0.0000013728151,0.00018882421,0.000003876602,0.00040035814],"genre_scores_gemma":[0.9995975,0.000023523111,0.000050601502,0.0000017415986,0.0000017847586,9.1523117e-7,0.0002512429,0.0000019522195,0.00007079788],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998492,0.000019062134,0.000019672934,0.000056369467,0.000029055336,0.000026620628],"domain_scores_gemma":[0.9986582,0.00035402292,0.00048270557,0.00013204027,0.00015758032,0.00021541183],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023971176,0.00012595393,0.00019659272,0.0016301047,0.00024496907,0.0005999134,0.00017937244,0.00018681817,0.0016980052],"category_scores_gemma":[0.001360352,0.000107852946,0.00015085597,0.0010703539,0.00023446108,0.00035977745,0.00047267776,0.00012986652,0.0003410799],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003255603,0.000004489925,0.9969618,0.0000052312375,0.000022317805,0.000025375393,0.000027309141,0.000091881724,0.001557483,0.000037368092,0.000019132627,0.0012150136],"study_design_scores_gemma":[0.0000010372837,0.0000121225485,0.99927825,8.2847794e-7,0.000005214226,0.000064831496,0.000052211002,0.00020997656,0.00021935186,0.000038033755,0.00011751006,7.674681e-7],"about_ca_topic_score_codex":0.0010250997,"about_ca_topic_score_gemma":0.0011634163,"teacher_disagreement_score":0.0016980052,"about_ca_system_score_codex":0.00012925979,"about_ca_system_score_gemma":0.00007261131,"threshold_uncertainty_score":0.005680442},"labels":[],"label_agreement":null},{"id":"W4401376403","doi":"10.3847/1538-4357/ad583e","title":"Unified Rapid Mass Transfer","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Mitacs","keywords":"Physics; Binary number; Arithmetic underflow; Binary star; Mass transfer; Astrophysics; Formalism (music); Roche lobe; Computational physics; Stars; Mechanics","score_opus":0.012225487191371235,"score_gpt":0.22275590315776903,"score_spread":0.2105304159663978,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401376403","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07445749,0.00035966423,0.90234685,0.00010061951,0.00010505537,0.00011053674,0.00024705124,0.0010345579,0.021238213],"genre_scores_gemma":[0.79955226,0.00031249205,0.19001207,0.00009909269,0.00013160855,0.0002387978,0.00020222853,0.00045125934,0.009000187],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997657,0.000056411543,0.000010017989,0.000047214315,0.0000832004,0.000037486556],"domain_scores_gemma":[0.99946684,0.00016261746,0.00007673444,0.00015669897,0.00008780305,0.00004934035],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005214002,0.0005747262,0.0005861419,0.0012100362,0.00046009707,0.0007572756,0.0011426988,0.00047021417,0.005302702],"category_scores_gemma":[0.0025049734,0.00035523807,0.0006701139,0.00048353805,0.00063828315,0.0013962687,0.0017346548,0.00073116535,0.0009248027],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018616719,0.0000919976,0.0037099,0.00024466094,0.000087556895,0.00044877786,0.00038122293,0.3198834,0.025639165,0.52658015,0.002492194,0.12025486],"study_design_scores_gemma":[0.00002454832,0.000048090697,0.0008791457,0.000015854153,0.00001738686,0.00013330695,0.000015838526,0.9234609,0.006266655,0.06463554,0.004474081,0.000028776252],"about_ca_topic_score_codex":0.000965807,"about_ca_topic_score_gemma":0.00073800224,"teacher_disagreement_score":0.005302702,"about_ca_system_score_codex":0.0006530427,"about_ca_system_score_gemma":0.00047522015,"threshold_uncertainty_score":0.017739296},"labels":[],"label_agreement":null},{"id":"W4401401418","doi":"10.3847/1538-4357/ad5be2","title":"Shoulder of Dust Rings Formed by Planet–Disk Interactions","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Academia Sinica","keywords":"Planet; Physics; Astrophysics; Millimeter; Radiative transfer; Planetesimal; Astronomy; Dust lane; Accretion (finance); Debris disk; Astrobiology; Planetary system; Stars; Star formation; Optics","score_opus":0.010901636104869045,"score_gpt":0.265317753627407,"score_spread":0.25441611752253795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401401418","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99644935,0.00007268463,0.0021624754,0.000020067193,0.0000051501,0.000005541842,0.00006585153,0.00010677868,0.0011122499],"genre_scores_gemma":[0.9995103,0.00000997137,0.00036531666,0.0000035387552,0.0000016348241,0.0000013407296,0.000029394427,0.000004923454,0.00007357481],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993634,0.000008221662,0.0000034019927,0.00001872685,0.000010105673,0.000023073113],"domain_scores_gemma":[0.99971324,0.00004908899,0.000105035644,0.00004249915,0.00002184387,0.00006829646],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013401623,0.00018285502,0.00021222726,0.00032362586,0.00030648406,0.00060981506,0.00029879363,0.00024358607,0.0013783324],"category_scores_gemma":[0.00042998575,0.00021786615,0.00039547696,0.00014548878,0.00035017324,0.00028396645,0.00053319073,0.0001870795,0.00017296083],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011667743,0.00025664017,0.39812928,0.0002067711,0.00040802968,0.0041293493,0.0009932157,0.33651477,0.22881244,0.005700143,0.0017195869,0.021963062],"study_design_scores_gemma":[0.00010535471,0.00018278534,0.33600286,0.000018605631,0.00009015368,0.0006969045,0.0002959451,0.6363481,0.021915559,0.0028140992,0.0014872968,0.000042320964],"about_ca_topic_score_codex":0.0014704886,"about_ca_topic_score_gemma":0.00061538856,"teacher_disagreement_score":0.0014704886,"about_ca_system_score_codex":0.00030171606,"about_ca_system_score_gemma":0.00014444445,"threshold_uncertainty_score":0.0046109557},"labels":[],"label_agreement":null},{"id":"W4401434608","doi":"10.3847/1538-4357/ad5099","title":"Faraday Tomography with CHIME: The “Tadpole” Feature G137+7","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Advanced Frequency and Time Standards","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; Okanagan College; McGill University; University of Calgary; Herzberg Institute of Astrophysics; University of British Columbia, Okanagan Campus; Dominion Astrophysical Observatory; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Division of Astronomical Sciences; HORIZON EUROPE European Research Council; Canada Foundation for Innovation; National Research Council Canada; Smithsonian Astrophysical Observatory","keywords":"Physics; Faraday effect; Polarization (electrochemistry); Faraday cage; Astrophysics; Spectral line; Astronomy; Magnetic field","score_opus":0.003551445191178258,"score_gpt":0.2242373673248008,"score_spread":0.22068592213362254,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401434608","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94673425,0.00030169263,0.016601564,0.00095291634,0.000051546132,0.000050311748,0.0034358583,0.0012962127,0.030575572],"genre_scores_gemma":[0.9843056,0.00009044053,0.010732272,0.00012682368,0.000009312485,0.000016166658,0.0018031271,0.00027596526,0.002640393],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999068,0.0000056680824,0.0000013421852,0.000019068451,0.00003209054,0.00003511338],"domain_scores_gemma":[0.9998908,0.000018872148,0.00001781698,0.000020691687,0.00002504506,0.000026836573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019511317,0.00023109031,0.00023142988,0.00053925987,0.00034793044,0.0006320734,0.00042034176,0.00038709788,0.00611901],"category_scores_gemma":[0.00023389107,0.00015391334,0.00020043632,0.00059049623,0.00041927682,0.00036438106,0.00060232455,0.0006476964,0.00077775755],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007107699,0.000107623615,0.035020333,0.00014382676,0.00009341455,0.0021234641,0.00061540905,0.009929785,0.90288985,0.006054057,0.009492554,0.032818798],"study_design_scores_gemma":[0.0003165906,0.00037021912,0.30688238,0.00009393657,0.00011951007,0.0020018304,0.0013587316,0.06755312,0.54502964,0.0070320033,0.06907887,0.00016321932],"about_ca_topic_score_codex":0.0058277175,"about_ca_topic_score_gemma":0.012404855,"teacher_disagreement_score":0.00611901,"about_ca_system_score_codex":0.00071094977,"about_ca_system_score_gemma":0.00027462532,"threshold_uncertainty_score":0.020470142},"labels":[],"label_agreement":null},{"id":"W4401465334","doi":"10.3847/1538-4357/ad53c1","title":"SCUBA-2 Ultra Deep Imaging EAO Survey (STUDIES). V. Confusion-limited Submillimeter Galaxy Number Counts at 450 μm and Data Release for the COSMOS Field","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University","funders":"National Science and Technology Council; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; National Research Foundation of Korea; Academia Sinica; National Natural Science Foundation of China; Science and Technology Facilities Council; National Research Foundation; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Astronomical Research Institute of Thailand; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; James Clerk Maxwell Telescope; Astrophysics; Galaxy; Advanced Camera for Surveys; Flux (metallurgy); Noise (video); Astronomy; Star formation; Image (mathematics); Artificial intelligence","score_opus":0.026262258259960976,"score_gpt":0.2836600511675734,"score_spread":0.25739779290761244,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401465334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7546887,0.00035192803,0.0053088716,0.00029996742,0.000054414395,0.0003216099,0.2129163,0.0021189172,0.023939302],"genre_scores_gemma":[0.6541068,0.000201643,0.014044039,0.00033845773,0.00011568765,0.00036657555,0.32188058,0.0005220733,0.008424132],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996923,0.000039464318,0.000027856133,0.00005573599,0.00012151056,0.00006311019],"domain_scores_gemma":[0.9985933,0.00011118098,0.0003709604,0.00030016116,0.00029647755,0.0003279564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065174914,0.00031899064,0.00021315747,0.002622274,0.00031454323,0.000587305,0.00045430075,0.0001694466,0.003428206],"category_scores_gemma":[0.0013765837,0.0002043506,0.00029176756,0.0022447233,0.00013102355,0.0003497122,0.00062324066,0.00020445095,0.0017633078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005239758,0.00012974582,0.84234375,0.00013241654,0.00013715788,0.00030941668,0.0003615328,0.0024647084,0.014807183,0.001336299,0.075552866,0.061900914],"study_design_scores_gemma":[0.000026041458,0.000018966135,0.98320794,0.000011037304,0.000015347325,0.00005641722,0.00003311338,0.0013322758,0.0014367839,0.0001478466,0.013700302,0.000013839498],"about_ca_topic_score_codex":0.026317338,"about_ca_topic_score_gemma":0.04324968,"teacher_disagreement_score":0.026317338,"about_ca_system_score_codex":0.00039866412,"about_ca_system_score_gemma":0.00046939045,"threshold_uncertainty_score":0.05232829},"labels":[],"label_agreement":null},{"id":"W4401465603","doi":"10.3847/1538-4357/ad54af","title":"BreakBRD Galaxies: Evolutionary Clues through an Analysis of Gas Content","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Universidad Nacional Autónoma de México; Space Telescope Science Institute; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science Foundation; Flatiron Health; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Content (measure theory); Galaxy; Astrophysics; Astronomy; Galaxy formation and evolution","score_opus":0.016792700367423377,"score_gpt":0.24592873011922678,"score_spread":0.22913602975180342,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401465603","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979538,0.00028201172,0.0002752111,0.000012735769,0.0000014344009,0.00000457292,0.00089312857,0.000021357586,0.00055573974],"genre_scores_gemma":[0.9985745,0.000052252013,0.00037621238,0.00000882069,0.000002771953,0.0000032069988,0.00083816814,0.00000416219,0.00013992902],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998548,0.000017613407,0.000008979941,0.000051223706,0.000029887844,0.000037461235],"domain_scores_gemma":[0.9993793,0.000082257175,0.00024265685,0.000053847816,0.00007341924,0.00016853886],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003325897,0.00017579552,0.00024214879,0.0023048948,0.0001693862,0.00064081146,0.00024514477,0.00022476862,0.0015875606],"category_scores_gemma":[0.00054504175,0.00014077377,0.00017319235,0.00094904756,0.0002475454,0.0003649947,0.0006083078,0.00017325066,0.00044276132],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060238228,0.0000099701,0.985025,0.000012305913,0.00002794339,0.00003523574,0.000100355166,0.000080498416,0.01162208,0.00004036474,0.000067857865,0.0029181119],"study_design_scores_gemma":[7.581384e-7,0.000010960951,0.9992619,0.0000015895772,0.0000035495991,0.000048311183,0.00006604868,0.00012786042,0.00031712014,0.00001916843,0.00014161527,0.0000011831778],"about_ca_topic_score_codex":0.0029457523,"about_ca_topic_score_gemma":0.003948438,"teacher_disagreement_score":0.0029457523,"about_ca_system_score_codex":0.00024131262,"about_ca_system_score_gemma":0.000064374035,"threshold_uncertainty_score":0.005857229},"labels":[],"label_agreement":null},{"id":"W4401583389","doi":"10.3847/1538-4357/ad596f","title":"Denser Environments Cultivate Larger Galaxies: A Comprehensive Study beyond the Local Universe with 3 Million Hyper Suprime-Cam Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Japan Society for the Promotion of Science; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; National Central University; Nuclear Safety and Security Commission; Washington Research Foundation; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; Eötvös Loránd Tudományegyetem; Academia Sinica; Los Alamos National Laboratory; Princeton University; University of Washington; Johns Hopkins University; Space Telescope Science Institute; National Science Foundation; Durham University; Japan Science and Technology Agency; John Templeton Foundation; Smithsonian Institution; Science Mission Directorate; Yale University; Queen's University Belfast; National Aeronautics and Space Administration","keywords":"Galaxy; Physics; Astrophysics; Universe; RADIUS; Galaxy formation and evolution; Effective radius; Astronomy","score_opus":0.007294979194110446,"score_gpt":0.20519033784916244,"score_spread":0.19789535865505198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401583389","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99879324,0.00019111802,0.00012788275,0.000033381504,7.691335e-7,0.0000024518283,0.00034835745,0.000012081127,0.00049070665],"genre_scores_gemma":[0.9985482,0.00014373483,0.000319571,0.00003310589,0.000008792944,0.000004502609,0.00068442983,0.000010312533,0.00024740992],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997973,0.000053832027,0.000009624426,0.000062371844,0.00003757802,0.00003933713],"domain_scores_gemma":[0.99887735,0.00021922936,0.00025671188,0.0002464467,0.00008543262,0.00031492228],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056704594,0.00020634476,0.00030516647,0.0010954869,0.00053078646,0.00065105193,0.00031735474,0.00015063936,0.0011511467],"category_scores_gemma":[0.0007965538,0.00015795878,0.00034987225,0.0012785431,0.00050909974,0.00062673487,0.0011295339,0.0002895115,0.00027373654],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007657169,0.000039635073,0.9863868,0.000023508726,0.000094705036,0.00016457557,0.0020201504,0.00018576752,0.0019506759,0.00031651242,0.00076893595,0.007972181],"study_design_scores_gemma":[0.0000014718172,0.000024815561,0.9979371,0.0000050602234,0.000015810614,0.00011044364,0.0003872183,0.00015959112,0.00016160264,0.0000757881,0.0011184969,0.0000026234075],"about_ca_topic_score_codex":0.006070659,"about_ca_topic_score_gemma":0.0091493605,"teacher_disagreement_score":0.006070659,"about_ca_system_score_codex":0.00021624469,"about_ca_system_score_gemma":0.00015634643,"threshold_uncertainty_score":0.012070656},"labels":[],"label_agreement":null},{"id":"W4401591848","doi":"10.3847/1538-4357/ad583c","title":"JWST Photometry of Globular Clusters in A2744. II. Luminosity and Color Distributions","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Globular cluster; Physics; Photometry (optics); Astrophysics; Astronomy; Blue straggler; Horizontal branch; Luminosity; Star cluster; Galaxy; Stars","score_opus":0.008213783668591837,"score_gpt":0.2335624498438117,"score_spread":0.22534866617521987,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401591848","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99842596,0.00003360398,0.00030786984,0.00003317753,0.0000011756916,0.000003227876,0.00031401656,0.00003295465,0.0008479984],"genre_scores_gemma":[0.9981206,0.000023874221,0.00046814655,0.000012128602,0.000002248722,0.0000034492225,0.0010088449,0.00001668784,0.0003439741],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998995,0.00001000142,0.0000036504262,0.000029902523,0.000031704792,0.000025160189],"domain_scores_gemma":[0.99954057,0.00008415079,0.00008857219,0.00006709412,0.00010575671,0.000113914124],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033432958,0.00018959245,0.00020011303,0.0009445956,0.00031817876,0.00046988195,0.00045945324,0.00028413575,0.0011671048],"category_scores_gemma":[0.00094609807,0.00022961266,0.0003464469,0.0006421871,0.0003605476,0.00044274825,0.00069295464,0.00022525285,0.0003780235],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016013192,0.00008380009,0.87112564,0.00004113218,0.00014266353,0.0002673429,0.00032356082,0.091423035,0.020355064,0.0024668816,0.0022131759,0.011397632],"study_design_scores_gemma":[0.000032858035,0.0000511579,0.873169,0.000009005103,0.00003057672,0.0001551347,0.00018590917,0.12053115,0.0035982616,0.00087840686,0.001333292,0.000025270423],"about_ca_topic_score_codex":0.027242916,"about_ca_topic_score_gemma":0.02986894,"teacher_disagreement_score":0.027242916,"about_ca_system_score_codex":0.0011100264,"about_ca_system_score_gemma":0.00035224445,"threshold_uncertainty_score":0.0541687},"labels":[],"label_agreement":null},{"id":"W4401734095","doi":"10.3847/1538-4357/ad57c2","title":"Observational Characteristics of Circumplanetary-mass-object Disks in the Era of James Webb Space Telescope","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Basic and Applied Basic Research Foundation of Guangdong Province; Alliance de recherche numérique du Canada; Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China","keywords":"Physics; James Webb Space Telescope; Astronomy; Spitzer Space Telescope; Telescope; Space (punctuation); Astrophysics","score_opus":0.019049342144471657,"score_gpt":0.24422680782194645,"score_spread":0.2251774656774748,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401734095","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998803,0.000055304456,0.00012341686,0.000006371762,9.1081597e-7,0.0000048865645,0.0005157733,0.000009872206,0.00048043893],"genre_scores_gemma":[0.9983651,0.000031303633,0.0002079551,0.0000041005,0.0000019372587,0.000003591881,0.0012506531,0.000004178736,0.0001311988],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980813,0.000023242717,0.000014047576,0.00007042897,0.000049609527,0.000034629033],"domain_scores_gemma":[0.999297,0.000120231205,0.00020933908,0.00007417437,0.00009343127,0.00020590224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036271694,0.0001612837,0.00011616012,0.0024924313,0.00033442967,0.00044337206,0.00024486773,0.00020230799,0.0008063156],"category_scores_gemma":[0.00097164325,0.00010835724,0.00015886372,0.001031035,0.00020946767,0.00034833848,0.00041132353,0.000098974764,0.00024566887],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005939094,0.000027934793,0.99051636,0.000008720454,0.000017977156,0.00005197217,0.000129719,0.00043212916,0.004062861,0.00008363843,0.00015467209,0.00445462],"study_design_scores_gemma":[7.5544983e-7,0.0000060274783,0.9992169,9.783391e-7,0.0000026626142,0.00002837463,0.000025832464,0.00040930742,0.00015723873,0.000014650833,0.00013617252,0.0000010968242],"about_ca_topic_score_codex":0.006013888,"about_ca_topic_score_gemma":0.011294989,"teacher_disagreement_score":0.006013888,"about_ca_system_score_codex":0.00036072824,"about_ca_system_score_gemma":0.00010505945,"threshold_uncertainty_score":0.011957765},"labels":[],"label_agreement":null},{"id":"W4401742696","doi":"10.3847/1538-4357/ad58bc","title":"The Nearly Universal Disk Galaxy Rotation Curve","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec; Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; Queen's University; Australian Government; Canadian Institute for Theoretical Astrophysics","keywords":"Galaxy rotation curve; Physics; Galaxy; Dark matter; Astrophysics; Rotation (mathematics); Surface brightness; Halo; Artificial intelligence; Computer science","score_opus":0.0057653318248892796,"score_gpt":0.21061035541139297,"score_spread":0.2048450235865037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401742696","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.73994654,0.0009813271,0.24823074,0.00031105228,0.00004865848,0.000049453927,0.0016111708,0.0013852465,0.007435797],"genre_scores_gemma":[0.98993427,0.000057903362,0.009174011,0.000027000646,0.000010089154,0.000006865923,0.00048404,0.000037048078,0.0002688565],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99946076,0.0001536927,0.000028110888,0.00023484469,0.00006082935,0.00006173885],"domain_scores_gemma":[0.9985669,0.00037648424,0.00015984375,0.0005039076,0.0003021441,0.000090711284],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011639805,0.000345281,0.00042874616,0.00073470204,0.0002938263,0.0007998453,0.0007045154,0.0003578035,0.0012524931],"category_scores_gemma":[0.005745704,0.00015999291,0.00031717628,0.00047695075,0.0006536415,0.0010586405,0.0005777414,0.00048671637,0.0003328076],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018094387,0.000036415433,0.18451062,0.00010283946,0.00010651201,0.00013022474,0.00013813168,0.6464984,0.0057177353,0.01566248,0.0040268926,0.14288884],"study_design_scores_gemma":[0.000006882628,0.000021910026,0.026614046,0.000029188817,0.000008868167,0.000065052365,0.000034947134,0.96287537,0.0018031894,0.0069836047,0.0015424077,0.000014513386],"about_ca_topic_score_codex":0.010655652,"about_ca_topic_score_gemma":0.008318669,"teacher_disagreement_score":0.010655652,"about_ca_system_score_codex":0.00081329216,"about_ca_system_score_gemma":0.0004206899,"threshold_uncertainty_score":0.021187246},"labels":[],"label_agreement":null},{"id":"W4401747016","doi":"10.3847/1538-4357/ad58db","title":"Flaring Stars in a Nontargeted Millimeter-wave Survey with SPT-3G","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Three-Speed Logic (Canada); Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University; Canadian Institute for Advanced Research","funders":"SLAC National Accelerator Laboratory; Fermilab; Laboratory Directed Research and Development; Australian Research Council; Horizon 2020 Framework Programme; University of California, Los Angeles; Argonne National Laboratory; U.S. Department of Energy; California Institute of Technology; European Commission; McGill University; University of Chicago; Office of Science; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; Jet Propulsion Laboratory; Centre National d’Etudes Spatiales","keywords":"Physics; Astrophysics; Stars; ROSAT; Flare; Sky; Galaxy; Astronomy; Telescope; Flare star; Population; K-type main-sequence star; T Tauri star","score_opus":0.018842775904711624,"score_gpt":0.2247502218856592,"score_spread":0.2059074459809476,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401747016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9866108,0.00013498582,0.0006173189,0.00003801496,0.000008258465,0.00003823431,0.011363825,0.00015292542,0.0010356875],"genre_scores_gemma":[0.9441173,0.0001309952,0.002287428,0.00012632008,0.00003463095,0.00006804035,0.052274752,0.00007794142,0.0008825845],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99933124,0.000058704627,0.000043618253,0.00018158108,0.0002604499,0.00012445395],"domain_scores_gemma":[0.99813616,0.00009229928,0.0007617981,0.00028815222,0.00031510484,0.00040655822],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047563956,0.0003634797,0.00044242592,0.0020807378,0.0002993782,0.00061611366,0.00045789347,0.0003341352,0.0012528903],"category_scores_gemma":[0.00085404154,0.00022505318,0.00042702368,0.0023040068,0.0001638714,0.0003171288,0.0010348018,0.00027210973,0.0011557735],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017242957,0.00007967267,0.9713208,0.00005319891,0.000116682364,0.00035624194,0.00022640207,0.00032288424,0.009475797,0.00005493894,0.003740183,0.014080783],"study_design_scores_gemma":[0.0000064368865,0.00002843814,0.9976871,0.0000035852268,0.000014655799,0.00013277897,0.000023396056,0.00024370162,0.00032256538,0.000009359194,0.0015254874,0.0000025933343],"about_ca_topic_score_codex":0.009243186,"about_ca_topic_score_gemma":0.017071927,"teacher_disagreement_score":0.009243186,"about_ca_system_score_codex":0.00036319738,"about_ca_system_score_gemma":0.00031162077,"threshold_uncertainty_score":0.018378794},"labels":[],"label_agreement":null},{"id":"W4401748130","doi":"10.3847/1538-4357/ad5540","title":"The Ultraviolet Luminosity Function at 0.6 &lt; z &lt; 1 from UVCANDELS","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"National Natural Science Foundation of China; Fundamental Research Funds for the Central Universities; Science and Technology Facilities Council; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Photometry (optics); Redshift; Astrophysics; Galaxy; Luminosity function; Ultraviolet; Luminosity; Astronomy; Optics; Stars","score_opus":0.006894481280251227,"score_gpt":0.20287080256125523,"score_spread":0.195976321281004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401748130","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96234465,0.00012302553,0.0017192415,0.00007447543,0.000011529728,0.000023583896,0.023556136,0.00037888673,0.011768468],"genre_scores_gemma":[0.9235374,0.0001156845,0.0024618253,0.00008413602,0.00002449175,0.000030756797,0.06123058,0.00008581723,0.012429419],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974316,0.000014148181,0.000008649163,0.00006625958,0.000106333726,0.000061459534],"domain_scores_gemma":[0.9993807,0.000043264532,0.00015156178,0.000067362205,0.0001644684,0.00019258531],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027158513,0.00025820083,0.0001710529,0.0021585617,0.0003424772,0.0008644373,0.00035088105,0.00017773124,0.0053974153],"category_scores_gemma":[0.0005563118,0.00012538246,0.00021291943,0.0010230327,0.00018416787,0.00025620568,0.0004428696,0.00021427416,0.0026761768],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011698979,0.00007543818,0.93057936,0.00003332988,0.000042173764,0.00014341889,0.00039766534,0.0010584842,0.0077078193,0.001071537,0.012525268,0.046248447],"study_design_scores_gemma":[0.000002958091,0.00001658169,0.9908083,0.000007856942,0.0000074662944,0.000058197355,0.000046210018,0.0009597295,0.0012968661,0.00009368186,0.0066973534,0.000004848769],"about_ca_topic_score_codex":0.022521583,"about_ca_topic_score_gemma":0.0267715,"teacher_disagreement_score":0.022521583,"about_ca_system_score_codex":0.0006304174,"about_ca_system_score_gemma":0.00033587182,"threshold_uncertainty_score":0.04478097},"labels":[],"label_agreement":null},{"id":"W4401769955","doi":"10.3847/1538-4357/ad5cee","title":"Constraining Cosmological Parameters Using the Splashback Radius of Galaxy Clusters","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Leverhulme Trust","keywords":"Physics; Astrophysics; Redshift; Galaxy cluster; Weak gravitational lensing; Galaxy; Cluster (spacecraft); Universe; RADIUS","score_opus":0.021699424559858408,"score_gpt":0.24638565235640125,"score_spread":0.22468622779654285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401769955","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99432313,0.0001205736,0.0039238185,0.00005523521,0.0000037157063,0.0000046833925,0.00020506856,0.0000827257,0.0012810918],"genre_scores_gemma":[0.9986028,0.000023659564,0.0012033798,0.0000065479558,0.0000018112438,0.0000016333414,0.00010859409,0.000012997822,0.000038538717],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998604,0.000043893753,0.0000064875985,0.00004879472,0.000022551469,0.000017911705],"domain_scores_gemma":[0.9987061,0.00057140505,0.00029346207,0.00018255289,0.00007971206,0.00016672687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059789495,0.0003261378,0.00037090867,0.0009026148,0.00033208908,0.00077194546,0.000533377,0.00032326014,0.0008957957],"category_scores_gemma":[0.0030023041,0.00029063653,0.00031047253,0.0005203575,0.000503595,0.0008535767,0.0007503379,0.00046767297,0.00016023108],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004822881,0.00011635952,0.47896302,0.00016546353,0.0003644239,0.00022001639,0.00042454712,0.4630166,0.026647322,0.012951133,0.0011945695,0.015454295],"study_design_scores_gemma":[0.000056911453,0.00007929552,0.19375288,0.000043512187,0.000090921865,0.00005987704,0.00014828218,0.78861374,0.00758228,0.008054859,0.0014599527,0.00005754047],"about_ca_topic_score_codex":0.010873878,"about_ca_topic_score_gemma":0.011084244,"teacher_disagreement_score":0.010873878,"about_ca_system_score_codex":0.0007702506,"about_ca_system_score_gemma":0.00031019148,"threshold_uncertainty_score":0.021621168},"labels":[],"label_agreement":null},{"id":"W4401821753","doi":"10.3847/1538-4357/ad5291","title":"The NANOGrav 15 yr Data Set: Chromatic Gaussian Process Noise Models for Six Pulsars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; University of British Columbia","funders":"H2020 Excellent Science; University of British Columbia Graduate School; H2020 European Research Council; Agence Nationale de la Recherche; National Aeronautics and Space Administration; Central Laser Facility, Science and Technology Facilities Council; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Pulsar; Noise (video); Achromatic lens; Data set; Chromatic scale; Algorithm; Astrophysics; Astronomy; Artificial intelligence; Optics; Computer science","score_opus":0.03515095553067807,"score_gpt":0.368624239063793,"score_spread":0.3334732835331149,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401821753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96801513,0.00016193182,0.0061425036,0.00042997065,0.000036763013,0.00006290156,0.021873228,0.0003948448,0.0028826864],"genre_scores_gemma":[0.9265918,0.00009957662,0.0044973064,0.00013705973,0.00003306143,0.0001024612,0.06721674,0.00015881432,0.0011631488],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9995179,0.00013913355,0.000043209606,0.00013987742,0.0001186788,0.000041180672],"domain_scores_gemma":[0.9974643,0.0015878159,0.0002296526,0.00038280818,0.00023087134,0.000104532344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0020376416,0.00042838094,0.0005015939,0.0011642706,0.0004218766,0.00070577004,0.0011196849,0.00076148217,0.0025055099],"category_scores_gemma":[0.0045777867,0.00020725494,0.0010073838,0.0013792496,0.00033435415,0.0006005719,0.00069354865,0.0006503093,0.0007042593],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001636015,0.0006314658,0.26095483,0.0003171294,0.0006702759,0.00074586313,0.00040747953,0.6391773,0.006877353,0.0089389905,0.03426661,0.045376718],"study_design_scores_gemma":[0.0003401398,0.00022667361,0.21325833,0.000051767707,0.00010701249,0.0002934516,0.00023446996,0.7637752,0.0035755914,0.0047879517,0.01323894,0.00011052384],"about_ca_topic_score_codex":0.01701945,"about_ca_topic_score_gemma":0.01499174,"teacher_disagreement_score":0.01701945,"about_ca_system_score_codex":0.0005958842,"about_ca_system_score_gemma":0.00036437344,"threshold_uncertainty_score":0.033840775},"labels":[],"label_agreement":null},{"id":"W4401825009","doi":"10.3847/1538-4357/ad496a","title":"GWSkyNet. II. A Refined Machine-learning Pipeline for Real-time Classification of Public Gravitational Wave Alerts","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; Indo-US Science and Technology Forum; Canada Research Chairs; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Physics; Gravitational wave; Classifier (UML); LIGO; False alarm; Artificial intelligence; Sky; Constant false alarm rate; Snapshot (computer storage); Pipeline (software); Machine learning; Astronomy; Computer science; Real-time computing","score_opus":0.03093823712933271,"score_gpt":0.32653696088112943,"score_spread":0.29559872375179674,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401825009","genre_codex":"software","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.16601756,0.0008229461,0.35039246,0.00088062143,0.0007803369,0.00082869333,0.016330231,0.45594534,0.00800178],"genre_scores_gemma":[0.5806261,0.00022274548,0.33914894,0.0009869789,0.00018074537,0.0008846842,0.058500454,0.0050187926,0.014430657],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993144,0.00009232226,0.000046215817,0.00026920723,0.0001764644,0.00010142093],"domain_scores_gemma":[0.9988148,0.0003494244,0.000085237494,0.00030293126,0.00034248328,0.00010518653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014910422,0.0016552435,0.0007053978,0.0016901257,0.000515733,0.0012365974,0.0028334754,0.0014586027,0.007855863],"category_scores_gemma":[0.004226463,0.00064265303,0.00070198777,0.0009063166,0.0005102178,0.0022336822,0.0014163987,0.0015980408,0.0060644965],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018747603,0.0008088907,0.017306827,0.00047386944,0.00034146284,0.0003956093,0.00028139094,0.09566157,0.02705804,0.0035212939,0.16064239,0.6916339],"study_design_scores_gemma":[0.00009505338,0.00017737948,0.003500481,0.000021718746,0.000025334362,0.000052103045,0.000040819854,0.97003996,0.011952057,0.0034248505,0.010631175,0.000038955626],"about_ca_topic_score_codex":0.013500257,"about_ca_topic_score_gemma":0.015760304,"teacher_disagreement_score":0.013500257,"about_ca_system_score_codex":0.0010247686,"about_ca_system_score_gemma":0.0015110342,"threshold_uncertainty_score":0.02684331},"labels":[],"label_agreement":null},{"id":"W4401868479","doi":"10.3847/1538-4357/ad6143","title":"Action-angle Variables for Axisymmetric Potentials via Birkhoff Normalization","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Target Tracking and Data Fusion in Sensor Networks","field":"Computer Science","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics","keywords":"Physics; Normalization (sociology); Rotational symmetry; Action (physics); Astrophysics; Classical mechanics; Astronomy; Mechanics; Quantum mechanics","score_opus":0.01989177091599804,"score_gpt":0.2653901882287351,"score_spread":0.24549841731273708,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401868479","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.04032669,0.00032255406,0.9279908,0.00016262809,0.00019299416,0.00010170971,0.00014388455,0.0009446655,0.029814027],"genre_scores_gemma":[0.6150583,0.0007211319,0.36854768,0.00032193508,0.00014195441,0.00036138666,0.00041385365,0.0029618067,0.011471965],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9992686,0.00022724153,0.000030102816,0.00004825993,0.00032759656,0.00009814428],"domain_scores_gemma":[0.99899703,0.00036340184,0.00012345027,0.00017205387,0.00024701582,0.00009705944],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014554462,0.00075564714,0.0005985179,0.0019710634,0.001107282,0.0014338667,0.0017626507,0.00056385854,0.0077480148],"category_scores_gemma":[0.0049826666,0.00038487904,0.0006016541,0.0013697493,0.0014007537,0.0026759722,0.0012358151,0.0013949807,0.0019333068],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008144692,0.00008551167,0.0010546134,0.0001282943,0.000033166292,0.00020780455,0.00018911115,0.14066085,0.006548256,0.8029541,0.0029845352,0.04507239],"study_design_scores_gemma":[0.000016703605,0.00002214648,0.00046259796,0.000041001986,0.0000066055127,0.00008156949,0.000067973604,0.77977186,0.0033128276,0.21134831,0.004827878,0.00004047548],"about_ca_topic_score_codex":0.0041247164,"about_ca_topic_score_gemma":0.0044476595,"teacher_disagreement_score":0.0077480148,"about_ca_system_score_codex":0.0012488135,"about_ca_system_score_gemma":0.0015350211,"threshold_uncertainty_score":0.025919676},"labels":[],"label_agreement":null},{"id":"W4401868518","doi":"10.3847/1538-4357/ad6602","title":"RRAT J1913+1330: An Extremely Variable and Puzzling Pulsar","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia, Okanagan Campus; University of British Columbia","funders":"Youth Innovation Promotion Association; Natural Science Foundation of Jiangsu Province; Government of Jiangsu Province; China Postdoctoral Science Foundation; Chinese Academy of Sciences; National Natural Science Foundation of China; Alexander von Humboldt-Stiftung","keywords":"Physics; Pulsar; Astrophysics; Astronomy; Variable star; Stars","score_opus":0.01605961673559091,"score_gpt":0.32040532638713265,"score_spread":0.30434570965154173,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401868518","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984862,0.00014225305,0.00051602937,0.000040120107,0.000012836663,0.000007886101,0.00025484178,0.000054763466,0.00048503012],"genre_scores_gemma":[0.99786633,0.000068885434,0.00085065165,0.00006976859,0.000040991883,0.000007360242,0.0009199088,0.000023267321,0.00015291167],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999026,0.0000057369066,0.000007701968,0.0000359045,0.00002301897,0.000024956042],"domain_scores_gemma":[0.9996381,0.000030057825,0.0001422049,0.000036813006,0.000030258172,0.00012255998],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020303264,0.00030287696,0.00046898992,0.0009420894,0.00086040125,0.0005693801,0.00037361943,0.00036820228,0.0006680052],"category_scores_gemma":[0.0002585208,0.00020456678,0.0002202684,0.0016536162,0.00037886068,0.00017506637,0.00046613818,0.00041869888,0.0003192876],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005210001,0.00018912576,0.7717348,0.00011959872,0.0001780295,0.006322234,0.0005380177,0.0005986384,0.19628808,0.0007356668,0.0019656247,0.020809237],"study_design_scores_gemma":[0.000021469566,0.00010265783,0.988983,0.000008233106,0.00005639903,0.0041342317,0.00013479494,0.0007652893,0.0030608245,0.00021577383,0.0025011864,0.00001621183],"about_ca_topic_score_codex":0.0018500754,"about_ca_topic_score_gemma":0.003088768,"teacher_disagreement_score":0.0018500754,"about_ca_system_score_codex":0.00030288965,"about_ca_system_score_gemma":0.00023300407,"threshold_uncertainty_score":0.0036786199},"labels":[],"label_agreement":null},{"id":"W4401885974","doi":"10.3847/1538-4357/ad5671","title":"Observations of Low and Intermediate Spectral Peak Blazars with the Imaging X-Ray Polarimetry Explorer","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Consejo Superior de Investigaciones Científicas; Japan Society for the Promotion of Science; Leibniz-Gemeinschaft; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; Marshall Space Flight Center; Korea Research Environment Open Network; Istituto Nazionale di Fisica Nucleare; Stockholms Universitet; Junta de Andalucía; National Astronomical Observatory of Japan; National Institutes of Natural Sciences; Nuclear Safety and Security Commission; Háskóli Íslands; Istituto Nazionale di Astrofisica; European Commission; Ministerio de Ciencia e Innovación; Centre National de la Recherche Scientifique; Max-Planck-Gesellschaft; California Institute of Technology; Turun Yliopisto; Aarhus Universitet; Academia Sinica; Universitetet i Oslo; Yale University; University of Crete; Instituto de Astrofísica de Andalucía; Ministry of Education, Culture, Sports, Science and Technology; Korea Institute of Science and Technology Information; Smithsonian Institution; National Radio Astronomy Observatory; Korea Institute of Science and Technology; Space Telescope Science Institute; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Agenzia Spaziale Italiana; National Science Foundation","keywords":"Physics; Blazar; Polarimetry; Polarization (electrochemistry); Astrophysics; Photon; X-ray; Electron; Astronomy; Gamma ray; Optics; Scattering; Nuclear physics","score_opus":0.008169897456440223,"score_gpt":0.21130653801052335,"score_spread":0.20313664055408312,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401885974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99436694,0.000077436634,0.0009607157,0.00004170896,0.0000026262662,0.000009885493,0.0004631166,0.000075479096,0.004002127],"genre_scores_gemma":[0.9978241,0.000057082147,0.0009197887,0.000021943126,0.000009863356,0.0000062191157,0.0007272569,0.000017503378,0.00041615567],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998971,0.000012324344,0.000003939871,0.000024990557,0.00003114595,0.000030515032],"domain_scores_gemma":[0.9997218,0.00005792968,0.00009751513,0.000027764285,0.000033452965,0.00006149527],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002836369,0.00028305233,0.00017421346,0.0009785924,0.00037212967,0.0005815404,0.00018062533,0.00020679933,0.0011532063],"category_scores_gemma":[0.00029305415,0.00013214955,0.00016013546,0.0005443242,0.00027179497,0.00020403381,0.00045743975,0.0004512885,0.0002557503],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00065792067,0.000118000644,0.8013694,0.000059842947,0.00010547049,0.0006488885,0.0007539854,0.0009157944,0.1736157,0.0012799703,0.0010208547,0.019454027],"study_design_scores_gemma":[0.00002527808,0.00006802397,0.98766965,0.000007805657,0.000030661915,0.00026478834,0.00015392914,0.00064288895,0.009721507,0.00018124853,0.0012260071,0.000008339563],"about_ca_topic_score_codex":0.0015887241,"about_ca_topic_score_gemma":0.0026173785,"teacher_disagreement_score":0.0015887241,"about_ca_system_score_codex":0.00020484101,"about_ca_system_score_gemma":0.00010018163,"threshold_uncertainty_score":0.003857851},"labels":[],"label_agreement":null},{"id":"W4401966951","doi":"10.3847/1538-4357/ad6147","title":"Should Zeros Count? Modeling the Galaxy–Globular Cluster Scaling Relation with(out) Zero-inflated Count Models","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; University of Toronto","keywords":"Physics; Globular cluster; Scaling; Galaxy; Astrophysics; Zero (linguistics); Cluster (spacecraft); Count data; Galaxy cluster; Astronomy; Statistics; Geometry","score_opus":0.017404919434050436,"score_gpt":0.22929546569804288,"score_spread":0.21189054626399245,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4401966951","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7749348,0.0007239595,0.21332265,0.0027331135,0.00015301506,0.00018019076,0.0011133362,0.00069157,0.006147509],"genre_scores_gemma":[0.9839325,0.00014807441,0.012432401,0.00028577386,0.000104236926,0.00014636325,0.0006097012,0.00010718881,0.002233795],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9975057,0.0013578235,0.00008882987,0.000588278,0.00020539403,0.00025403735],"domain_scores_gemma":[0.9636049,0.027667487,0.003803801,0.0020836354,0.0018696958,0.0009703468],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.011677486,0.0011322227,0.0013423484,0.0019474975,0.0010717236,0.0029714394,0.00394471,0.0024230105,0.0033811794],"category_scores_gemma":[0.050400216,0.0007084075,0.0013904652,0.0012465233,0.0028100384,0.0037411721,0.0014840192,0.0023425962,0.0006881282],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032442855,0.00021038532,0.06085914,0.00012810752,0.00017445334,0.00049924315,0.0008989596,0.78329545,0.00088646944,0.13323188,0.004791795,0.014699779],"study_design_scores_gemma":[0.000017754353,0.000030508721,0.0030487317,0.000022737331,0.0000217222,0.000058904374,0.00005614598,0.9660876,0.00011380067,0.030048905,0.00047278593,0.000020467864],"about_ca_topic_score_codex":0.017751267,"about_ca_topic_score_gemma":0.009852246,"teacher_disagreement_score":0.017751267,"about_ca_system_score_codex":0.00269949,"about_ca_system_score_gemma":0.0007244684,"threshold_uncertainty_score":0.061757207},"labels":[],"label_agreement":null},{"id":"W4402129432","doi":"10.3847/1538-4357/ad5963","title":"Abundances of Planetary Nebulae and Evolved Stars: Iron and Sulfur Depletion, and Carbon and Nitrogen Enrichment, in Low- and Intermediate-mass Stellar Populations in the Milky Way","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Planetary nebula; Physics; Asymptotic giant branch; Astrophysics; Stars; Abundance (ecology); Milky Way; Nucleosynthesis; Astronomy; Biology","score_opus":0.01163249239853903,"score_gpt":0.23087218896114559,"score_spread":0.21923969656260656,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402129432","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9997583,0.00006797029,0.000013447616,0.0000036315816,3.6473514e-7,3.6604743e-7,0.00005666627,8.6006764e-7,0.00009842565],"genre_scores_gemma":[0.99961555,0.000032780114,0.000036616417,0.0000056580884,0.0000010879278,0.0000010908191,0.00015474447,0.0000011363869,0.00015128587],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990344,0.000009862405,0.0000104535175,0.000040079805,0.000018358502,0.000017784712],"domain_scores_gemma":[0.9997608,0.00002807439,0.00008325969,0.00001605775,0.000048528975,0.00006327856],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002075466,0.00010570984,0.00025060956,0.0009412353,0.00026480758,0.0005396825,0.00025454027,0.00022937632,0.00067114504],"category_scores_gemma":[0.00043754416,0.00009751406,0.00015942703,0.00040359693,0.0003420483,0.00027330394,0.00043459176,0.00012814754,0.00020892054],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000065065404,0.000011098814,0.99469274,0.000008305275,0.000027167976,0.00005011555,0.00017077735,0.00003824859,0.0036568327,0.000027270175,0.000017355249,0.0012351166],"study_design_scores_gemma":[0.0000010620324,0.000019735067,0.9991109,0.0000016003746,0.0000058363344,0.000080197846,0.00017998164,0.00006594901,0.0003910727,0.00001983787,0.00012299707,8.6340316e-7],"about_ca_topic_score_codex":0.0034381528,"about_ca_topic_score_gemma":0.004243005,"teacher_disagreement_score":0.0034381528,"about_ca_system_score_codex":0.00025677058,"about_ca_system_score_gemma":0.00013089742,"threshold_uncertainty_score":0.006836295},"labels":[],"label_agreement":null},{"id":"W4402140882","doi":"10.3847/1538-4357/ad6444","title":"Water Evolution and Inventories of Super-Earths Orbiting Late M Dwarfs","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs","keywords":"Physics; Astronomy; Brown dwarf; Astrophysics; Exoplanet; White dwarf; Stars; Massive compact halo object; Stellar evolution; Astrobiology","score_opus":0.006878442085713704,"score_gpt":0.2037845625410301,"score_spread":0.1969061204553164,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402140882","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99879384,0.00001723554,0.00030428398,0.000036869682,0.0000024029446,0.0000043661344,0.00036287896,0.000025088832,0.0004530417],"genre_scores_gemma":[0.9988539,0.000016669579,0.00031516366,0.000011417013,0.0000013341406,0.0000064679903,0.0005404945,0.000012620187,0.00024194043],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999928,0.0000143756,0.000004212098,0.000020469957,0.000008452189,0.000024498817],"domain_scores_gemma":[0.9995685,0.00013851716,0.00007262914,0.000046890927,0.000048302325,0.00012516584],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002682633,0.00034633616,0.00044373234,0.00039025082,0.00045483938,0.0006828542,0.00067139394,0.000847674,0.0020457162],"category_scores_gemma":[0.0011622703,0.0003069601,0.0007924542,0.0003843245,0.00049337896,0.00073181436,0.00056469004,0.00049678405,0.00019149629],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024077436,0.000103064616,0.14851406,0.000027977061,0.00012012829,0.00019572595,0.00011681882,0.84411424,0.003516148,0.0011415641,0.00042025908,0.0014893056],"study_design_scores_gemma":[0.00009194924,0.00013952343,0.03513209,0.000010515297,0.00003333479,0.000053752206,0.00017846495,0.96189195,0.0011806533,0.0007553695,0.0005078285,0.000024607394],"about_ca_topic_score_codex":0.026526283,"about_ca_topic_score_gemma":0.013250824,"teacher_disagreement_score":0.026526283,"about_ca_system_score_codex":0.0007211616,"about_ca_system_score_gemma":0.00042665665,"threshold_uncertainty_score":0.052743733},"labels":[],"label_agreement":null},{"id":"W4402151369","doi":"10.3847/1538-4357/ad683f","title":"Erratum: “A Search for IceCube Sub-TeV Neutrinos Correlated with Gravitational-wave Events Detected By LIGO/Virgo” (2023, ApJ, 959, 96)","year":2024,"lang":"en","type":"erratum","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Fonds Wetenschappelijk Onderzoek; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Vetenskapsrådet; University of Wisconsin-Madison; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; National Research Foundation; Michigan State University; University of Oxford; Chiba University; Santen; Compute Canada; Marquette University","keywords":"LIGO; Physics; Neutrino; Gravitational wave; Astronomy; Astrophysics; Particle physics","score_opus":0.010461459389203235,"score_gpt":0.23291739288739516,"score_spread":0.22245593349819193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402151369","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.015573921,0.004671647,0.004721399,0.09355903,0.76127726,0.00028741875,0.047418717,0.0034549905,0.06903559],"genre_scores_gemma":[0.07704958,0.008120178,0.026366169,0.07558142,0.10342264,0.0004221792,0.08052226,0.0039505376,0.62456506],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9993037,0.00010058808,0.00010094932,0.00011891867,0.00033368013,0.000042259217],"domain_scores_gemma":[0.99560946,0.0012092508,0.00065485627,0.00030720021,0.0019477763,0.00027149083],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011277103,0.001518623,0.00051527674,0.0031715399,0.0021082968,0.0016293073,0.0011474709,0.0015214209,0.028737787],"category_scores_gemma":[0.009763492,0.00039699656,0.00049383816,0.0022438874,0.0006899958,0.00087834155,0.0007768543,0.0017596561,0.01621312],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000783076,0.000020780342,0.0014375307,0.00006547214,0.000010599076,0.00036750946,0.000030835257,0.000086780594,0.00024383592,0.00043344163,0.9878395,0.009385289],"study_design_scores_gemma":[0.000056415887,0.000075060336,0.008825287,0.00018244021,0.000046502664,0.00085138914,0.00017549019,0.0005662635,0.0012316724,0.0006509764,0.98730487,0.00003372816],"about_ca_topic_score_codex":0.018176982,"about_ca_topic_score_gemma":0.026171735,"teacher_disagreement_score":0.028737787,"about_ca_system_score_codex":0.001308283,"about_ca_system_score_gemma":0.0017001154,"threshold_uncertainty_score":0.096137464},"labels":[],"label_agreement":null},{"id":"W4402168127","doi":"10.3847/1538-4357/ad5834","title":"BP3M: Bayesian Positions, Parallaxes, and Proper Motions Derived from the Hubble Space Telescope and Gaia Data","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Natural Sciences and Engineering Research Council of Canada; Ministerio de Ciencia e Innovación; European Commission; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Hubble space telescope; Astronomy; Astrophysics; Space observatory; Spitzer Space Telescope; Space (punctuation); Telescope; Stars; Infrared","score_opus":0.017344680988173072,"score_gpt":0.23969490610209623,"score_spread":0.22235022511392316,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402168127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.46133235,0.000618313,0.4057967,0.0006429177,0.00006949897,0.00023294233,0.0815042,0.039735135,0.0100679705],"genre_scores_gemma":[0.66260046,0.00011860949,0.24239613,0.00017962234,0.000059713333,0.00017313678,0.09059223,0.0022305562,0.0016495157],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9990753,0.00015850618,0.00003566418,0.00023592838,0.00038579336,0.00010887044],"domain_scores_gemma":[0.9981888,0.00035802118,0.00039258137,0.00047171625,0.00039244734,0.00019646175],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0024074123,0.0007343338,0.0004026489,0.0027003991,0.0005252087,0.001218888,0.0010222212,0.00065663934,0.0039760205],"category_scores_gemma":[0.00668895,0.0006282338,0.0009937354,0.0017628864,0.0003024839,0.00089357333,0.0017395382,0.0009335971,0.0031080951],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00083406875,0.00023047735,0.43234524,0.00035664125,0.0007036315,0.00021459056,0.000500389,0.19502409,0.027667182,0.010090063,0.07268543,0.25934815],"study_design_scores_gemma":[0.00011567844,0.00008124647,0.23178063,0.00007257393,0.00009256208,0.00015914359,0.000102661295,0.72273844,0.012152295,0.011471207,0.021085907,0.0001476239],"about_ca_topic_score_codex":0.033466026,"about_ca_topic_score_gemma":0.028926017,"teacher_disagreement_score":0.033466026,"about_ca_system_score_codex":0.0011439143,"about_ca_system_score_gemma":0.0014294514,"threshold_uncertainty_score":0.066542506},"labels":[],"label_agreement":null},{"id":"W4402239989","doi":"10.3847/1538-4357/ad6140","title":"Inferring Host-galaxy Properties of LIGO–Virgo–KAGRA’s Black Holes","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Department of Atomic Energy, Government of India; National Science Foundation","keywords":"Physics; LIGO; Galaxy; Astronomy; Astrophysics; Supermassive black hole; Black hole (networking); Gravitational wave","score_opus":0.020032211104700208,"score_gpt":0.30099699032238075,"score_spread":0.28096477921768054,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402239989","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99892104,0.00001799918,0.00065452565,0.000008115637,6.826068e-7,0.00000217758,0.00017567222,0.000039138642,0.00018069551],"genre_scores_gemma":[0.99958915,0.000004602043,0.00024087852,0.0000020767143,9.1369816e-7,4.3653188e-7,0.00013783413,0.0000035187743,0.000020604837],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998872,0.000027772903,0.00000550133,0.000033336066,0.000017910888,0.000028334885],"domain_scores_gemma":[0.99909735,0.00024244824,0.00031133465,0.00013437707,0.00008084225,0.00013363635],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00064618204,0.00019514741,0.00019904283,0.0017370592,0.00015891356,0.00045145952,0.00035804868,0.00034467535,0.0007241071],"category_scores_gemma":[0.0023150668,0.00018404692,0.00026826456,0.00062504516,0.00024706934,0.000402509,0.00029512955,0.00012926596,0.00020095933],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012292682,0.000027643966,0.9741319,0.000007944412,0.00007184325,0.000053362433,0.00006980686,0.01630164,0.005372637,0.00044234228,0.00011936926,0.0032786678],"study_design_scores_gemma":[0.000014840181,0.00003303654,0.8740655,0.000004449826,0.000029201674,0.00006439522,0.0000630325,0.122286946,0.0027556892,0.00044346089,0.00022972467,0.000009594251],"about_ca_topic_score_codex":0.0070576244,"about_ca_topic_score_gemma":0.007601473,"teacher_disagreement_score":0.0070576244,"about_ca_system_score_codex":0.0005343095,"about_ca_system_score_gemma":0.00012366314,"threshold_uncertainty_score":0.014033139},"labels":[],"label_agreement":null},{"id":"W4402281812","doi":"10.3847/1538-4357/ad5c64","title":"SN 2024ggi in NGC 3621: Rising Ionization in a Nearby, Circumstellar-material-interacting Type II Supernova","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":30,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"H2020 European Research Council; University of California Observatories; Horizon 2020 Framework Programme; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Villum Fonden; National Astronomical Research Institute of Thailand; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Canada Research Chairs; University of California, Santa Cruz; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; Science and Technology Facilities Council; University of Toronto; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Radiative transfer; Stars; Ionization; Emission spectrum; Spectral line; Astronomy; Ion","score_opus":0.012075874392783067,"score_gpt":0.2521819909507658,"score_spread":0.24010611655798275,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402281812","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993388,0.000041711024,0.00013235727,0.000012945303,0.0000024724834,0.0000031210975,0.00010494074,0.0000318117,0.0003317955],"genre_scores_gemma":[0.9994912,0.000012476165,0.00013475156,0.0000059731274,0.0000022731533,0.0000016426069,0.00024457133,0.0000033583754,0.00010370261],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993277,0.0000072246394,0.0000031156285,0.000020377885,0.000013260435,0.000023351378],"domain_scores_gemma":[0.99986625,0.0000090533595,0.000033020668,0.000012969204,0.000010450517,0.00006820347],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014062795,0.0005404748,0.00037330276,0.00043740697,0.000517184,0.00051718886,0.00039142746,0.0004652095,0.0007554049],"category_scores_gemma":[0.0001914198,0.00015005359,0.0004676206,0.00031758993,0.00023250787,0.00018494586,0.00040790622,0.00023947259,0.00019477078],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005458371,0.00014005895,0.9224005,0.00002652303,0.00012927962,0.004268428,0.00019771191,0.014365185,0.053233813,0.00037096202,0.0005585309,0.0037632443],"study_design_scores_gemma":[0.000018513272,0.00020998654,0.967949,0.00000408798,0.000045616565,0.0011792581,0.00020237567,0.025805335,0.003432354,0.0002298967,0.0009031029,0.000020387415],"about_ca_topic_score_codex":0.023811713,"about_ca_topic_score_gemma":0.020054853,"teacher_disagreement_score":0.023811713,"about_ca_system_score_codex":0.000934829,"about_ca_system_score_gemma":0.00019699747,"threshold_uncertainty_score":0.047346175},"labels":[],"label_agreement":null},{"id":"W4402378313","doi":"10.3847/1538-4357/ad5a7c","title":"SN 2022oqm: A Bright and Multipeaked Calcium-rich Transient","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research, Development and Innovation Office; Stockholms Universitet; Turun Yliopisto; Háskóli Íslands; Agencia Estatal de Investigación; Universitetet i Oslo; Magyar Tudományos Akadémia; Queen's University; Aarhus Universitet; European Commission; Space Telescope Science Institute; Queen's University Belfast; Science and Technology Facilities Council; National Centre for Supercomputing Applications; National Aeronautics and Space Administration; Nemzeti Kutatási, Fejlesztési és Innovaciós Alap; University of Illinois at Urbana-Champaign; Nuclear Safety and Security Commission; Hungarian Scientific Research Fund; Heising-Simons Foundation; Villum Fonden; National Science Foundation","keywords":"Physics; Ejecta; Astrophysics; Supernova; Luminosity; Galaxy; Light curve; White dwarf; Population; Photosphere; Astronomy; Spectral line; Stars","score_opus":0.011974010169018485,"score_gpt":0.2412083690186822,"score_spread":0.22923435884966373,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402378313","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984666,0.00004846583,0.0001596866,0.000022736196,0.0000042335964,0.000005322176,0.00017185202,0.000015576128,0.0011055678],"genre_scores_gemma":[0.9990017,0.000020065632,0.00017465917,0.000021106176,0.0000059365166,0.0000018855967,0.00034504113,0.0000043069135,0.00042532332],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999504,0.0000019716615,0.0000019590345,0.000012614777,0.000012951459,0.000020126814],"domain_scores_gemma":[0.9998938,0.0000055552523,0.000024583964,0.000006219482,0.000014709423,0.000055209624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000102423226,0.00025964496,0.0001523982,0.00054557115,0.00033453968,0.0003240995,0.00018199452,0.000273089,0.0010499711],"category_scores_gemma":[0.00014064202,0.00007212306,0.00016292054,0.00029336332,0.00016576244,0.00015663338,0.00040760575,0.00013699767,0.00026663468],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034178505,0.00006894257,0.9214151,0.000035882378,0.000039732266,0.0060078013,0.00019295432,0.000627908,0.056869343,0.0006922782,0.0008867023,0.0128214825],"study_design_scores_gemma":[0.000009803333,0.00013271673,0.986349,0.00000781985,0.000016831109,0.004937354,0.00020459795,0.0014689155,0.003713492,0.00021473931,0.0029356438,0.000009048176],"about_ca_topic_score_codex":0.0040178197,"about_ca_topic_score_gemma":0.00839614,"teacher_disagreement_score":0.0040178197,"about_ca_system_score_codex":0.00034100364,"about_ca_system_score_gemma":0.0001049432,"threshold_uncertainty_score":0.00798887},"labels":[],"label_agreement":null},{"id":"W4402426698","doi":"10.3847/1538-4357/ad698d","title":"Multiwavelength Investigation of γ-Ray Source MGRO J1908+06 Emission Using Fermi-LAT, VERITAS and HAWC","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Coordinación de la Investigación Científica; Los Alamos National Laboratory; Goddard Space Flight Center; Office of Science; Office of National Higher Education Science Research and Innovation Policy Council; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; Japan Aerospace Exploration Agency; Benemérita Universidad Autónoma de Puebla; Institute for Cosmic Ray Research, University of Tokyo; Centre National de la Recherche Scientifique; U.S. Department of Energy; Smithsonian Institution; Vetenskapsrådet; Agenzia Spaziale Italiana; Generalitat Valenciana; National Energy Research Scientific Computing Center; Laboratory Directed Research and Development; National Science Foundation; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Istituto Nazionale di Astrofisica; Natural Sciences and Engineering Research Council of Canada; Barnard College; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Universities Space Research Association; Consejo Nacional de Ciencia y Tecnología","keywords":"Physics; Fermi Gamma-ray Space Telescope; Astrophysics; Pulsar; Telescope; Pulsar wind nebula; Cherenkov radiation; Astronomy; Cherenkov Telescope Array; Observatory; Nebula; Stars; Detector; Optics","score_opus":0.014100625430370802,"score_gpt":0.23637155950840366,"score_spread":0.22227093407803286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402426698","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969215,0.00006922391,0.0005128861,0.000020157375,0.0000032698856,0.000007208558,0.0005406576,0.00008872697,0.0018363559],"genre_scores_gemma":[0.997285,0.000034089706,0.0014975172,0.000015362226,0.0000059350537,0.0000053704516,0.00077646255,0.000025165076,0.00035511114],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989307,0.000008222803,0.000003714964,0.00003688067,0.00002786348,0.000030192092],"domain_scores_gemma":[0.999767,0.000030911313,0.00007625791,0.000038483104,0.000034011526,0.00005334419],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024931264,0.00023652834,0.00024309003,0.0011642716,0.00041014102,0.00035505847,0.0003057425,0.00018205667,0.0011353608],"category_scores_gemma":[0.00020083308,0.00016630752,0.000331176,0.0005982179,0.00014225772,0.0002021522,0.00034513324,0.00018979903,0.00021961788],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00082373567,0.00017202411,0.6508772,0.00007514833,0.0002120395,0.0014543246,0.00050099177,0.0041524842,0.3071987,0.0009034241,0.0010642587,0.032565683],"study_design_scores_gemma":[0.000020169711,0.00009106842,0.98092616,0.000009772986,0.000057314224,0.00032961776,0.00013467913,0.007540541,0.008836989,0.00010699836,0.0019318692,0.000014803949],"about_ca_topic_score_codex":0.006580417,"about_ca_topic_score_gemma":0.018084394,"teacher_disagreement_score":0.006580417,"about_ca_system_score_codex":0.00039400917,"about_ca_system_score_gemma":0.00014661178,"threshold_uncertainty_score":0.013084233},"labels":[],"label_agreement":null},{"id":"W4402454546","doi":"10.3847/1538-4357/ad5da7","title":"Revisiting Physical Parameters of the Benchmark Brown Dwarf LHS 6343 C through a Hubble Space Telescope/WFC3 Secondary-eclipse Observation","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Brown dwarf; Eclipse; Hubble space telescope; Astronomy; Astrophysics; Wide Field Camera 3; Space (punctuation); Galaxy; Stars","score_opus":0.018168241445019422,"score_gpt":0.24594033110194877,"score_spread":0.22777208965692936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402454546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9960246,0.000047982765,0.0005034439,0.0000389062,0.0000039297315,0.000007954145,0.0018982359,0.00017211022,0.0013029025],"genre_scores_gemma":[0.99670476,0.00001909631,0.0007379023,0.000026822716,0.0000043981486,0.000004023217,0.0023191231,0.00003772518,0.00014611552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999907,0.0000073494834,0.0000035550765,0.000032124437,0.000028084092,0.000021798012],"domain_scores_gemma":[0.9997514,0.000022895565,0.000044180157,0.000040632138,0.00006525015,0.00007566883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033073899,0.0002801658,0.00024860929,0.0006190847,0.00048437633,0.0004646263,0.0002833658,0.00030448523,0.00068613316],"category_scores_gemma":[0.00033558632,0.00013849277,0.00038954517,0.00053723797,0.00018191697,0.0002485408,0.00027387412,0.00029476485,0.0003623815],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025688348,0.00014040711,0.8904587,0.000066111,0.00012599079,0.0005639315,0.00039499934,0.011070259,0.07885859,0.00033323054,0.0037927476,0.013938137],"study_design_scores_gemma":[0.000015869357,0.000024611616,0.9762784,0.00000887026,0.000023584624,0.00007841033,0.000071553666,0.018510763,0.0036670188,0.00007520223,0.0012360358,0.00000951462],"about_ca_topic_score_codex":0.06712047,"about_ca_topic_score_gemma":0.11299449,"teacher_disagreement_score":0.06712047,"about_ca_system_score_codex":0.00089553033,"about_ca_system_score_gemma":0.0004002826,"threshold_uncertainty_score":0.13345957},"labels":[],"label_agreement":null},{"id":"W4402456224","doi":"10.3847/1538-4357/ad5cf2","title":"Studying Binary Formation under Dynamical Friction Using Hill’s Problem","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Electromagnetic Launch and Propulsion Technology","field":"Engineering","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Binary number; Dynamical friction; Astrophysics; Binary star; Astronomy; Statistical physics; Classical mechanics; Stars","score_opus":0.009807085467724087,"score_gpt":0.217342849541071,"score_spread":0.20753576407334692,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402456224","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8944081,0.00053457986,0.070839174,0.001322061,0.0001546504,0.00010230925,0.00025244095,0.0000775263,0.032309186],"genre_scores_gemma":[0.98928225,0.00012511208,0.0065707173,0.00012306671,0.000032428416,0.000045724508,0.00007670577,0.000025517349,0.0037183992],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998253,0.000059211467,0.000009014608,0.00002676981,0.000025670286,0.000054055214],"domain_scores_gemma":[0.9988642,0.00058228365,0.00022437776,0.00008282469,0.00007033122,0.00017601067],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076013076,0.00039065897,0.0008718021,0.00060267485,0.00067653175,0.00087299536,0.0008999149,0.0012477712,0.003446967],"category_scores_gemma":[0.0031322842,0.00033412184,0.0006904583,0.00041414396,0.0014342034,0.0017697975,0.0011856406,0.0007681462,0.00024388469],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000065902845,0.00006569138,0.0059221736,0.00005750424,0.000039989412,0.00025053043,0.0001311606,0.9085042,0.0011324455,0.08078529,0.0010346677,0.0020103662],"study_design_scores_gemma":[0.000029165521,0.000016468812,0.0007890959,0.0000060144107,0.00000346991,0.000034995624,0.000041209598,0.98970103,0.00013600876,0.008960819,0.0002734234,0.000008255026],"about_ca_topic_score_codex":0.009447956,"about_ca_topic_score_gemma":0.002865947,"teacher_disagreement_score":0.009447956,"about_ca_system_score_codex":0.0009751832,"about_ca_system_score_gemma":0.0005622839,"threshold_uncertainty_score":0.018785954},"labels":[],"label_agreement":null},{"id":"W4402659177","doi":"10.3847/1538-4357/adb622","title":"Superclustering with the Atacama Cosmology Telescope and Dark Energy Survey. II. Anisotropic Large-scale Coherence in Hot Gas, Galaxies, and Dark Matter","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"SLAC National Accelerator Laboratory; Integrated Electronics Engineering Center, Binghamton University; European Regional Development Fund; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Science; University of Illinois at Urbana-Champaign; National Institute of Standards and Technology; Institut de Física d'Altes Energies; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Agencia Nacional de Investigación y Desarrollo; Generalitat de Catalunya; University of Sussex; University of Toronto; National Aeronautics and Space Administration; University College London; Flatiron Health; National Energy Research Scientific Computing Center; High Energy Physics; Deutsche Forschungsgemeinschaft; Argonne National Laboratory; Centres de Recerca de Catalunya; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Government of Ontario; University of Portsmouth; Canadian Institute for Advanced Research; Ohio State University; Ministério da Ciência, Tecnologia e Inovação; Lawrence Berkeley National Laboratory; Financiadora de Estudos e Projetos; University of Pennsylvania; Ministerio de Ciencia e Innovación; European Commission; U.S. Department of Energy; Princeton University; Fermilab; National Science Foundation; Simons Foundation; Compute Canada; University of Chicago","keywords":"Physics; Astrophysics; Dark matter; Cosmology; Dark energy; Cosmic microwave background; South Pole Telescope; Weak gravitational lensing; Galaxy; Galaxy cluster; Redshift; Halo; Baryon; Anisotropy","score_opus":0.005131782454998448,"score_gpt":0.19949169432102964,"score_spread":0.1943599118660312,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402659177","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9854936,0.0001290264,0.0029194066,0.00015654432,0.000017003998,0.000028449796,0.0064489404,0.0004216676,0.004385459],"genre_scores_gemma":[0.98538035,0.000046147296,0.0063647144,0.000062862324,0.000024109902,0.000029528494,0.007278884,0.000100955614,0.0007123928],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997236,0.000046314795,0.000009537485,0.000080836624,0.00009742374,0.000042364514],"domain_scores_gemma":[0.9988651,0.0001092076,0.00036676988,0.00029624192,0.00013901592,0.00022379392],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006706595,0.00029971378,0.00025357452,0.0012572674,0.0003484996,0.0005364492,0.00045949026,0.00021726852,0.001489977],"category_scores_gemma":[0.0009219403,0.00022453963,0.0003687218,0.001183331,0.00023864112,0.00033391677,0.0008161375,0.00036054812,0.00045205123],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002598705,0.00008523991,0.94269437,0.000040493378,0.00032837244,0.00017853537,0.0003097021,0.0045434632,0.020950248,0.0019674595,0.0059613753,0.022680867],"study_design_scores_gemma":[0.000016153988,0.000016211245,0.9752236,0.000008123076,0.000019223973,0.000054607444,0.00007920862,0.0198178,0.0021111243,0.00046034518,0.0021813586,0.0000122949095],"about_ca_topic_score_codex":0.01445766,"about_ca_topic_score_gemma":0.022666786,"teacher_disagreement_score":0.01445766,"about_ca_system_score_codex":0.00038255804,"about_ca_system_score_gemma":0.00027977373,"threshold_uncertainty_score":0.028747022},"labels":[],"label_agreement":null},{"id":"W4402692340","doi":"10.3847/1538-4357/ad615a","title":"Nitrogen Abundance Distribution in the Inner Milky Way","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; Astrophysics Division; New York University Abu Dhabi; California Institute of Technology; National Aeronautics and Space Administration; York University; West Virginia University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Milky Way; Astrophysics; Galactic plane; Galaxy; Astronomy; Galactic Center; Galactic halo; Halo","score_opus":0.009051232763871656,"score_gpt":0.24248730327814494,"score_spread":0.2334360705142733,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402692340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963915,0.000036735823,0.00003511225,0.0000021968567,3.2775097e-7,4.1557962e-7,0.000057598452,0.000004212962,0.00022410258],"genre_scores_gemma":[0.99946636,0.000034702247,0.00011519198,0.000003881535,0.0000014467628,0.0000013130656,0.00024194292,0.0000032401206,0.0001320253],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998584,0.000009430221,0.000007145251,0.000066389424,0.000031381685,0.000027341013],"domain_scores_gemma":[0.99972254,0.000021695034,0.000118945485,0.000025883326,0.00005430049,0.000056543973],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000130172,0.00015171242,0.00026362058,0.001153482,0.00022740668,0.0004207394,0.00022264592,0.0001344686,0.00048269072],"category_scores_gemma":[0.00028047265,0.00010497604,0.00017170033,0.0006488931,0.00028354712,0.00026324132,0.00060762174,0.000073845324,0.00011868834],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007441815,0.0000136621675,0.983183,0.00001020647,0.000054373824,0.00016959434,0.0003236334,0.0002353408,0.011161478,0.000054442942,0.000059854858,0.004659906],"study_design_scores_gemma":[0.0000016298646,0.000021550508,0.9987262,0.0000019800286,0.000009269015,0.00007936254,0.00009541377,0.00017766832,0.0005554754,0.000014054084,0.000315372,0.0000020251812],"about_ca_topic_score_codex":0.0067059146,"about_ca_topic_score_gemma":0.008601817,"teacher_disagreement_score":0.0067059146,"about_ca_system_score_codex":0.0003413074,"about_ca_system_score_gemma":0.00012905855,"threshold_uncertainty_score":0.013333738},"labels":[],"label_agreement":null},{"id":"W4402693357","doi":"10.3847/1538-4357/ad684a","title":"CANUCS: An Updated Mass and Magnification Model of A370 with JWST","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Javna Agencija za Raziskovalno Dejavnost RS; Canadian Space Agency; National Research Foundation; Space Telescope Science Institute; Canarie; Canadian Foundation for AIDS Research; Danmarks Grundforskningsfond; National Aeronautics and Space Administration","keywords":"Physics; Galaxy; Redshift; James Webb Space Telescope; Astrophysics; Advanced Camera for Surveys; Stars; Algorithm; Hubble space telescope; Computer science","score_opus":0.008074232265901513,"score_gpt":0.2089098535075613,"score_spread":0.2008356212416598,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402693357","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.82659644,0.0008925222,0.10226321,0.0012244283,0.00009672879,0.00019261289,0.0023676,0.0010545905,0.06531183],"genre_scores_gemma":[0.9806342,0.00020465591,0.00781946,0.000109491986,0.00006542681,0.00008200351,0.00076900993,0.00020907186,0.010106653],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996675,0.000033907618,0.000008683011,0.00007068181,0.00012243673,0.00009683187],"domain_scores_gemma":[0.9995827,0.000042370863,0.0000743149,0.000059094218,0.00013183798,0.00010969653],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042258037,0.00083325687,0.00059907115,0.0013610572,0.0009647433,0.0013254421,0.002667439,0.000847846,0.004084918],"category_scores_gemma":[0.0013671571,0.00038899636,0.00092616375,0.00061709154,0.0009557314,0.0011327816,0.00075320277,0.00047831752,0.0012454184],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018319684,0.00007657316,0.07998974,0.00009524324,0.00014011243,0.0006934031,0.0007866348,0.75097924,0.012388504,0.11910357,0.010439336,0.025124377],"study_design_scores_gemma":[0.00003403151,0.00003657338,0.02332276,0.000021074336,0.00004048721,0.00015455096,0.000073813426,0.9548544,0.000795872,0.013611189,0.007004155,0.000051119805],"about_ca_topic_score_codex":0.28420353,"about_ca_topic_score_gemma":0.14439906,"teacher_disagreement_score":0.28420353,"about_ca_system_score_codex":0.006872413,"about_ca_system_score_gemma":0.0014906292,"threshold_uncertainty_score":0.5650985},"labels":[],"label_agreement":null},{"id":"W4402748370","doi":"10.3847/1538-4357/ad5a98","title":"An Untargeted Search for Radio-emitting Tidal Disruption Events in the VAST Pilot Survey","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Australian Research Council; Natural Sciences and Engineering Research Council of Canada; Israel Science Foundation; United States - Israel Binational Science Foundation; National Science Foundation","keywords":"Physics; Astronomy; Astrophysics; Astrobiology","score_opus":0.027661271494716515,"score_gpt":0.29810058149087887,"score_spread":0.27043930999616234,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402748370","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99469393,0.00004442737,0.0041608103,0.000023528482,0.000001983003,0.000041004518,0.00027685537,0.0000763115,0.000681169],"genre_scores_gemma":[0.9953471,0.000019486115,0.0041438034,0.0000124013395,0.0000016225665,0.000013431507,0.00026118197,0.000005546238,0.00019541619],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996805,0.000121372,0.000014828938,0.00006870794,0.0000702803,0.00004432139],"domain_scores_gemma":[0.9985311,0.0006529082,0.000301649,0.0001840644,0.00016920008,0.00016111883],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009307226,0.00012890481,0.00018513869,0.0009539634,0.00022128237,0.00040378745,0.00046381008,0.0001759805,0.00065874046],"category_scores_gemma":[0.003092578,0.0001544308,0.0002650162,0.0005655996,0.00021599636,0.00024939608,0.0006584856,0.000109246066,0.00014121488],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00027063634,0.00013181326,0.89313424,0.000072197945,0.0001476679,0.00066607306,0.00037473545,0.032926958,0.013415281,0.0014850992,0.0009156903,0.056459602],"study_design_scores_gemma":[0.00013011304,0.00090724864,0.7388429,0.00003617926,0.00018899496,0.0010904315,0.0005831165,0.24481916,0.007114668,0.0022632135,0.0039612516,0.00006265635],"about_ca_topic_score_codex":0.010308656,"about_ca_topic_score_gemma":0.019321539,"teacher_disagreement_score":0.010308656,"about_ca_system_score_codex":0.0002636945,"about_ca_system_score_gemma":0.0006132606,"threshold_uncertainty_score":0.020497322},"labels":[],"label_agreement":null},{"id":"W4402748720","doi":"10.3847/1538-4357/ad6317","title":"The Not-so Dramatic Effect of Advective Flows on Gas Accretion","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Accretion (finance); Advection; Astrophysics; Accretion disc; Astronomy; Thermodynamics","score_opus":0.005159349043215113,"score_gpt":0.2466412798287244,"score_spread":0.2414819307855093,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402748720","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951191,0.00027275347,0.0015704533,0.00014119907,0.000029741177,0.0000035808891,0.000065254026,0.00009179555,0.0027060108],"genre_scores_gemma":[0.9994373,0.000057545094,0.0002942396,0.00001237568,0.0000039318597,0.000001148027,0.000024231467,0.000007657131,0.00016160113],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999348,0.000011746381,0.0000043697714,0.000013827334,0.000013070935,0.000022148148],"domain_scores_gemma":[0.99938583,0.0003328713,0.00008147279,0.000067546665,0.000042780117,0.000089464054],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015827858,0.0003416704,0.00018335329,0.00019231183,0.00024107323,0.0007140903,0.0003176638,0.0002937406,0.0017476876],"category_scores_gemma":[0.0015768748,0.00014104505,0.00026507987,0.000102634796,0.00052211905,0.00056013255,0.0006128664,0.0005720284,0.000114298266],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008598448,0.00045324312,0.080287054,0.0004104453,0.0002730247,0.0013306726,0.00034842532,0.5537054,0.30981076,0.019265505,0.001540787,0.031714726],"study_design_scores_gemma":[0.000065057946,0.00031986702,0.04789837,0.000045042707,0.000072243216,0.00027728462,0.00015730089,0.87689525,0.06735466,0.0047252304,0.002142149,0.00004761961],"about_ca_topic_score_codex":0.0014042712,"about_ca_topic_score_gemma":0.0007012997,"teacher_disagreement_score":0.0017476876,"about_ca_system_score_codex":0.0002543547,"about_ca_system_score_gemma":0.00015621932,"threshold_uncertainty_score":0.0058466196},"labels":[],"label_agreement":null},{"id":"W4402843084","doi":"10.3847/1538-4357/ad643d","title":"Probing the Connection between IceCube Neutrinos and MOJAVE AGN","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Alliance de recherche numérique du Canada; Santen; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Fonds Wetenschappelijk Onderzoek; Nvidia; Marquette University","keywords":"Physics; Neutrino; Blazar; Astrophysics; Active galactic nucleus; Photon; Neutrino detector; Astronomy; Gamma ray; Galaxy; Neutrino oscillation; Nuclear physics","score_opus":0.011614146122760162,"score_gpt":0.22964252006729,"score_spread":0.21802837394452984,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402843084","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979309,0.000067779045,0.00052991055,0.000016585134,0.0000065548174,0.0000063169396,0.00067715376,0.000022502132,0.0007422982],"genre_scores_gemma":[0.9965796,0.00004652122,0.0008797899,0.000014121633,0.000017709828,0.000010320254,0.0021860306,0.000014460807,0.000251458],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995969,0.00009687296,0.000023409031,0.00012390359,0.00007613281,0.00008289611],"domain_scores_gemma":[0.99790907,0.0006825101,0.0008312962,0.00025188018,0.00018351307,0.00014175165],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00082070247,0.00024294663,0.00026591646,0.0011371641,0.0002513454,0.00091455394,0.00020611152,0.00023771844,0.0007641849],"category_scores_gemma":[0.0021832543,0.00018146378,0.00033710737,0.0009915801,0.00023112644,0.00027608682,0.0006185896,0.00036382882,0.00015977201],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016457782,0.00003690709,0.98918587,0.000009995013,0.00015493068,0.000068887246,0.00009958227,0.00084535335,0.005357607,0.0001323606,0.00019976764,0.0037441186],"study_design_scores_gemma":[0.000002856515,0.000032920434,0.99673814,0.0000035124408,0.000025482845,0.000059019803,0.000051240775,0.0015021815,0.0010706234,0.000047575722,0.0004630338,0.0000033788383],"about_ca_topic_score_codex":0.0046659308,"about_ca_topic_score_gemma":0.006396525,"teacher_disagreement_score":0.0046659308,"about_ca_system_score_codex":0.00025648528,"about_ca_system_score_gemma":0.00025503972,"threshold_uncertainty_score":0.009277582},"labels":[],"label_agreement":null},{"id":"W4402847277","doi":"10.3847/1538-4357/ad6606","title":"The Strength of Bisymmetric Modes in SDSS-IV/MaNGA Barred Galaxy Kinematics","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; University of California, Santa Cruz; Ohio State University; National Science Foundation; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Kinematics; Galaxy; Astronomy; Barred spiral galaxy; Type-cD galaxy; Galaxy formation and evolution; Classical mechanics","score_opus":0.011084179284826202,"score_gpt":0.2427626192465764,"score_spread":0.23167843996175022,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402847277","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99424547,0.000038728595,0.00492305,0.000029423261,0.000003347159,0.0000052251407,0.00021957258,0.00013725308,0.00039795076],"genre_scores_gemma":[0.99844605,0.0000066219595,0.0011295595,0.0000035111957,0.0000015161842,0.0000018411927,0.0003335111,0.000017106695,0.000060393737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996092,0.00013195594,0.000019533454,0.00013547247,0.00007522897,0.000028728398],"domain_scores_gemma":[0.9983193,0.0005088241,0.00048453527,0.00035582337,0.00017286873,0.00015862024],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00120376,0.00027477252,0.00019773045,0.0008576894,0.00031870123,0.00076290977,0.00033905508,0.00019076114,0.0008168159],"category_scores_gemma":[0.0030076928,0.00020461905,0.00035728424,0.00037953755,0.00052711274,0.0004181632,0.0006403106,0.0003007468,0.00023796632],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025100328,0.000063179265,0.87628114,0.000025076102,0.00011783162,0.00010695459,0.00028401415,0.09299616,0.009982378,0.0018357841,0.0005613051,0.017495144],"study_design_scores_gemma":[0.000013982488,0.000043422126,0.6031189,0.0000116938645,0.000020011215,0.00009082337,0.00013797602,0.39176437,0.0024291354,0.001716059,0.0006282629,0.00002544387],"about_ca_topic_score_codex":0.010175113,"about_ca_topic_score_gemma":0.010256867,"teacher_disagreement_score":0.010175113,"about_ca_system_score_codex":0.0004594997,"about_ca_system_score_gemma":0.00023183713,"threshold_uncertainty_score":0.020231783},"labels":[],"label_agreement":null},{"id":"W4402890164","doi":"10.3847/1538-4357/ad5fee","title":"Combined Pre-supernova Alert System with KamLAND and Super-Kamiokande","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Neutrino Physics Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Japan Society for the Promotion of Science; Horizon 2020 Framework Programme; Institute for Basic Science; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Ministry of Education, Culture, Sports, Science and Technology; Science and Technology Facilities Council; National Research Foundation; U.S. Department of Energy; European Commission; Western Canada Research Grid; National Natural Science Foundation of China; National Science Foundation; Compute Canada; National Research Foundation of Korea; Narodowym Centrum Nauki","keywords":"Physics; Supernova; Neutrino; Super-Kamiokande; Type II supernova; Neutrino detector; Astrophysics; Detector; Neutrino astronomy; Particle physics; Astronomy; Solar neutrino; Neutrino oscillation","score_opus":0.009350825495132739,"score_gpt":0.25099891379591344,"score_spread":0.2416480883007807,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402890164","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7681965,0.0017429993,0.17708771,0.00076905225,0.0005311726,0.0008039799,0.0031804573,0.03104974,0.016638394],"genre_scores_gemma":[0.91296816,0.00017264721,0.07763677,0.00044667142,0.00011423283,0.00019736307,0.0034127163,0.00020195247,0.004849437],"study_design_codex":"design_other","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9991128,0.00013782967,0.00006521706,0.0002750794,0.0002679694,0.0001410654],"domain_scores_gemma":[0.9987947,0.00012721537,0.00013548388,0.00024530923,0.0004715996,0.00022564233],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014930328,0.00070121617,0.0009282977,0.0016302544,0.00044202965,0.0008499706,0.00089162105,0.0008935482,0.0026184383],"category_scores_gemma":[0.0010795641,0.00039394418,0.00045030247,0.00068634603,0.00026962563,0.0012673163,0.00186059,0.00067260856,0.0010786159],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0060136956,0.0008771205,0.30460587,0.00078137836,0.0011879147,0.0042836405,0.000990659,0.010037184,0.3077785,0.0075885095,0.03493645,0.3209191],"study_design_scores_gemma":[0.0010258356,0.0036445695,0.18336804,0.00020375094,0.0016382764,0.00363301,0.0005556385,0.3515735,0.31766006,0.0063884016,0.12973133,0.0005776327],"about_ca_topic_score_codex":0.001086159,"about_ca_topic_score_gemma":0.0019480749,"teacher_disagreement_score":0.0026184383,"about_ca_system_score_codex":0.00040548603,"about_ca_system_score_gemma":0.0007341757,"threshold_uncertainty_score":0.008759499},"labels":[],"label_agreement":null},{"id":"W4402893672","doi":"10.3847/1538-4357/ad64d0","title":"A Multiwavelength Study to Decipher the 2017 Flare of the Blazar OJ 287","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy; Smithsonian Institution; National Science Foundation","keywords":"Physics; Blazar; Flare; DECIPHER; Astrophysics; Astronomy; Solar flare; Genetics; Gamma ray; Biology","score_opus":0.011074534131355526,"score_gpt":0.25381629722160415,"score_spread":0.2427417630902486,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4402893672","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983046,0.00011424939,0.00012173667,0.00003575824,0.0000052680116,0.000009582218,0.00019961204,0.000007104369,0.0012020634],"genre_scores_gemma":[0.9986362,0.00010436292,0.00023864866,0.00003598482,0.00002174178,0.0000038175494,0.0004461551,0.0000068508475,0.0005061952],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994695,0.0000025561944,0.0000017470642,0.0000121206,0.000014017045,0.000022564307],"domain_scores_gemma":[0.9998636,0.000010329369,0.000048832168,0.0000071452073,0.000019033401,0.000050935774],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009916038,0.00013331242,0.0001710221,0.00083528046,0.00039115144,0.00042455626,0.00013993718,0.00019511615,0.00080311566],"category_scores_gemma":[0.00015959813,0.0000864637,0.000171384,0.00052060705,0.0002090668,0.00019702809,0.00031182938,0.00036689566,0.00022347922],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030902374,0.00032430486,0.9134387,0.00007533831,0.00009724355,0.0034445105,0.0019396662,0.000302593,0.053411033,0.0003791094,0.0013000575,0.024978476],"study_design_scores_gemma":[0.000002236564,0.000027862547,0.9982723,0.00000417177,0.000006830642,0.00021782651,0.00035660694,0.00011118182,0.0002583317,0.000020358602,0.0007194311,0.000002848462],"about_ca_topic_score_codex":0.011393875,"about_ca_topic_score_gemma":0.025490265,"teacher_disagreement_score":0.011393875,"about_ca_system_score_codex":0.00032975478,"about_ca_system_score_gemma":0.00020184806,"threshold_uncertainty_score":0.02265513},"labels":[],"label_agreement":null},{"id":"W4403045549","doi":"10.3847/1538-4357/ad6905","title":"Massive White Dwarfs in the 100 pc Sample: Magnetism, Rotation, Pulsations, and the Merger Fraction","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":23,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Nuclear Safety and Security Commission; Canadian Institute for Theoretical Astrophysics; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Dartmouth College; Ohio State University; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Science Foundation","keywords":"Physics; White dwarf; Rotation (mathematics); Astrophysics; Astronomy; Magnetism; Sample (material); Stars; Stellar rotation; Condensed matter physics; Geometry","score_opus":0.009108456486540812,"score_gpt":0.2385038144859359,"score_spread":0.2293953579993951,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403045549","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9951461,0.00006319617,0.00022165998,0.0000324889,8.55385e-7,0.000006804084,0.0037347844,0.000031548178,0.0007625666],"genre_scores_gemma":[0.9952388,0.00003756297,0.00016192136,0.0000065118593,0.0000019219158,0.0000048423194,0.0039936607,0.000008387869,0.0005464549],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998746,0.0000145006925,0.0000049698747,0.00003405459,0.00004471237,0.000027140046],"domain_scores_gemma":[0.99968505,0.000051462604,0.00007050155,0.00004445968,0.00006394591,0.00008449631],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001807773,0.00018181518,0.00021682172,0.0008493339,0.00029656183,0.00043270117,0.00030743724,0.00009949815,0.002922181],"category_scores_gemma":[0.00087703776,0.00011122314,0.00017471635,0.0008578104,0.00013175095,0.00022304856,0.0003245686,0.000112845686,0.00043657405],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000049611237,0.000012795405,0.9940619,0.000004403932,0.00003271113,0.000050517414,0.000063940795,0.0006276408,0.0009439808,0.000088473396,0.00072878535,0.0033351288],"study_design_scores_gemma":[0.0000036289737,0.000011265127,0.99689037,0.0000012196157,0.000010230394,0.000045508266,0.00006440214,0.0018626625,0.00029819456,0.000038474318,0.00077040493,0.000003554343],"about_ca_topic_score_codex":0.28436977,"about_ca_topic_score_gemma":0.34253255,"teacher_disagreement_score":0.28436977,"about_ca_system_score_codex":0.0008073262,"about_ca_system_score_gemma":0.0003771754,"threshold_uncertainty_score":0.5654291},"labels":[],"label_agreement":null},{"id":"W4403074617","doi":"10.3847/1538-4357/ad675b","title":"The Peculiar Radio Evolution of the Tidal Disruption Event ASASSN-19bt","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Science and Technology Facilities Council; Nuclear Safety and Security Commission; National Research Foundation; Commonwealth Scientific and Industrial Research Organisation; Australian Government; York University; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Astrophysics; Event (particle physics); Astronomy","score_opus":0.006058589571538856,"score_gpt":0.23068154717044853,"score_spread":0.22462295759890968,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403074617","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987185,0.000041340943,0.00012642163,0.00001422364,0.000005725404,0.000003854478,0.0002285677,0.00000804042,0.0008532968],"genre_scores_gemma":[0.9987153,0.000026487503,0.00016073276,0.000011149522,0.000006259298,0.0000031014124,0.00077998027,0.000003668782,0.0002933509],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999348,0.000005897738,0.0000038033834,0.000015756215,0.000018481449,0.000021200403],"domain_scores_gemma":[0.99973875,0.00001292588,0.00008595253,0.00001938884,0.00004302964,0.000100006844],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013046428,0.00014739734,0.00020347392,0.00051155157,0.00038443092,0.0003541695,0.00017170967,0.00015760254,0.0006149178],"category_scores_gemma":[0.00022658124,0.00008221483,0.00015221564,0.00043895497,0.00024570918,0.00014166185,0.00045661026,0.00021407606,0.00019817815],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003460473,0.000063302214,0.9413502,0.000031267584,0.00005965506,0.0012723003,0.0005012187,0.0010258227,0.04474991,0.00034424633,0.00064048555,0.009615498],"study_design_scores_gemma":[0.000004406294,0.00005705005,0.9963903,0.000004059605,0.000008295299,0.00025528416,0.00018293869,0.00067024387,0.000692756,0.00005316716,0.0016762066,0.0000053528966],"about_ca_topic_score_codex":0.0065568653,"about_ca_topic_score_gemma":0.015700769,"teacher_disagreement_score":0.0065568653,"about_ca_system_score_codex":0.00047598107,"about_ca_system_score_gemma":0.00012520922,"threshold_uncertainty_score":0.013037384},"labels":[],"label_agreement":null},{"id":"W4403092950","doi":"10.3847/1538-4357/ad686a","title":"The Observational and Numerical Analysis of the Rayleigh–Taylor Instability beneath a Hedgerow Prominence","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Irish Centre for High-End Computing; Ministerio de Ciencia e Innovación; Royal Swedish Academy of Sciences; Trinity College Dublin; Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Queen's University; Irish Research Council; European Research Council; Science Foundation Ireland; Queen's University Belfast","keywords":"Physics; Rayleigh–Taylor instability; Instability; Observational study; Rayleigh scattering; Astrophysics; Astronomy; Mechanics; Optics; Medicine","score_opus":0.013254669167685206,"score_gpt":0.2462646569390786,"score_spread":0.2330099877713934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403092950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984876,0.000015396086,0.00058173726,0.000027215168,0.000002385105,0.0000043770765,0.00005912221,0.000032466258,0.00078959065],"genre_scores_gemma":[0.99937314,0.0000055380183,0.0005087061,0.000002903659,0.0000012974835,0.000003075952,0.00004457426,0.0000034616394,0.000057266312],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99993527,0.00001577968,0.0000033983379,0.000013586703,0.000013917886,0.000017952656],"domain_scores_gemma":[0.9995158,0.00023260673,0.00008160236,0.00004552966,0.00005290153,0.0000715759],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025811198,0.00019336116,0.00021150448,0.00041436433,0.00043935934,0.0003394856,0.0005055279,0.00039491785,0.0009950915],"category_scores_gemma":[0.0012980952,0.00016795499,0.000353983,0.00026601713,0.00041436273,0.0002398867,0.00033266866,0.0003351814,0.00006725956],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023652607,0.00015163791,0.0722496,0.00006251987,0.000084002364,0.00068248325,0.00022109125,0.90859425,0.009846926,0.0022220046,0.0004136816,0.005235244],"study_design_scores_gemma":[0.000027251814,0.000045294833,0.014873035,0.0000032399926,0.000008970023,0.000033655797,0.000040104587,0.9839482,0.0006771288,0.00022950396,0.00010645622,0.0000070626693],"about_ca_topic_score_codex":0.017579634,"about_ca_topic_score_gemma":0.008927676,"teacher_disagreement_score":0.017579634,"about_ca_system_score_codex":0.0006052863,"about_ca_system_score_gemma":0.0002893299,"threshold_uncertainty_score":0.034954667},"labels":[],"label_agreement":null},{"id":"W4403092983","doi":"10.3847/1538-4357/ad6a1b","title":"The Lower Limit of Dynamical Black Hole Masses Detectable in Virgo Compact Stellar Systems Using the JWST/NIRSpec IFU","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Canadian Space Agency; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Limit (mathematics); Astronomy; Young stellar object; Galaxy; Star formation","score_opus":0.010465193643385533,"score_gpt":0.2300891440044277,"score_spread":0.21962395036104218,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403092983","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9927261,0.000062517356,0.0046970374,0.000040161656,0.000005650416,0.000007816298,0.00073558994,0.00036552103,0.0013596467],"genre_scores_gemma":[0.9951568,0.000013636902,0.0035087522,0.000011578037,0.0000044376525,0.0000048030447,0.0011774859,0.00003216097,0.00009043531],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997527,0.000033335717,0.000008451448,0.00008844765,0.00005288138,0.00006408675],"domain_scores_gemma":[0.9990908,0.00016510295,0.00019810729,0.00028726226,0.00010452909,0.00015420212],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00072151324,0.0004099108,0.0002899753,0.00084694166,0.00043841885,0.00097526726,0.0006389737,0.00050504046,0.0008320838],"category_scores_gemma":[0.0024099422,0.00018209242,0.00045525425,0.0004429893,0.00043241217,0.00071822066,0.0005316325,0.00034611963,0.00031388027],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003442212,0.000112639216,0.8713878,0.0000807271,0.00017875756,0.00025845238,0.0004866624,0.058975745,0.038839664,0.0033782404,0.0014228025,0.02453431],"study_design_scores_gemma":[0.000015023703,0.00007478941,0.6703672,0.000039346916,0.00007724477,0.00018937688,0.00020767053,0.31094143,0.014522392,0.001769121,0.0017489045,0.00004748793],"about_ca_topic_score_codex":0.010631254,"about_ca_topic_score_gemma":0.011485622,"teacher_disagreement_score":0.010631254,"about_ca_system_score_codex":0.00049577124,"about_ca_system_score_gemma":0.00020737234,"threshold_uncertainty_score":0.021138787},"labels":[],"label_agreement":null},{"id":"W4403158229","doi":"10.3847/1538-4357/ad67d1","title":"Radio Scrutiny of the X-Ray-weak Tail of Low-mass Active Galactic Nuclei: A Novel Signature of High-Eddington Accretion?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Science Foundation","keywords":"Physics; Astrophysics; Active galactic nucleus; Accretion (finance); Astronomy; Accretion disc; Quasar; Galaxy","score_opus":0.008177733428058259,"score_gpt":0.22406225735589036,"score_spread":0.2158845239278321,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403158229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993106,0.00009372936,0.00014328897,0.000012009091,0.0000017723481,0.0000021504109,0.00007426697,0.000005741904,0.0003564247],"genre_scores_gemma":[0.9996278,0.000035883717,0.00010813532,0.000016431912,0.00000910493,0.0000020869086,0.00007912163,0.0000021719795,0.00011928578],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999876,0.00002604961,0.00001075467,0.000040871993,0.000019339937,0.000027000366],"domain_scores_gemma":[0.99877125,0.0002451971,0.00053422677,0.00012830272,0.00012535379,0.00019563605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003853442,0.00016671128,0.00016492984,0.0010121192,0.00020358045,0.0006250184,0.00029255,0.00023008227,0.0010412099],"category_scores_gemma":[0.0009437329,0.00008296626,0.0001033969,0.0003856992,0.0003906024,0.0002900154,0.0004482237,0.0002199496,0.000251448],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010166913,0.00003174834,0.9808358,0.000012375738,0.000020675281,0.00020988345,0.000165656,0.000027914462,0.01582596,0.000041211493,0.000050485334,0.0026765144],"study_design_scores_gemma":[0.0000017122536,0.000058105572,0.99819,0.0000024939577,0.000008467306,0.00048745974,0.00016012909,0.00007577983,0.00087665586,0.000019104766,0.0001181103,0.0000019338643],"about_ca_topic_score_codex":0.0005266369,"about_ca_topic_score_gemma":0.0006960754,"teacher_disagreement_score":0.0010412099,"about_ca_system_score_codex":0.00008033805,"about_ca_system_score_gemma":0.00004850482,"threshold_uncertainty_score":0.0034831762},"labels":[],"label_agreement":null},{"id":"W4403159987","doi":"10.3847/1538-4357/ad73d4","title":"Inferring Cosmological Parameters on SDSS via Domain-generalized Neural Networks and Light-cone Simulations","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Brookhaven National Laboratory; Samsung; Carnegie Mellon University; Korea Institute of Science and Technology; Korea Institute for Advancement of Technology; York University; Office of Science; Princeton University; Alfred P. Sloan Foundation; University of Washington; College of Engineering, Michigan State University; Johns Hopkins University; Ohio State University; National Research Foundation; Korea Institute of Science and Technology Information; Harvard University; National Science Foundation; Lawrence Berkeley National Laboratory; Ministry of Science and ICT, South Korea; National Research Foundation of Korea; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; U.S. Department of Energy","keywords":"Physics; Artificial neural network; Galaxy; Omega; Sigma; Robustness (evolution); Artificial intelligence; Algorithm; Minkowski space; Machine learning; Astrophysics; Computer science; Astronomy; Mathematical physics; Quantum mechanics","score_opus":0.011529374007981897,"score_gpt":0.23066908008332337,"score_spread":0.21913970607534147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403159987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.89459795,0.0001567674,0.100381516,0.00042317755,0.000028146467,0.000047121088,0.0008081752,0.0015204985,0.0020365592],"genre_scores_gemma":[0.9779158,0.000032586573,0.020224387,0.00008811651,0.000012787485,0.000027010323,0.001108623,0.000051875224,0.0005386575],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99968815,0.00015507765,0.000010274664,0.00006573456,0.000046597623,0.000034234577],"domain_scores_gemma":[0.9981115,0.0012118019,0.00013592915,0.0002312504,0.00020794294,0.000101649544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012288643,0.0006773081,0.00058161997,0.0006263771,0.00031393624,0.0007246811,0.0012663516,0.0006666489,0.0011608513],"category_scores_gemma":[0.0059572104,0.00039142036,0.0006083672,0.00047633782,0.0007365791,0.0008259991,0.0007814662,0.0010537299,0.00021545951],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000041416988,0.000022833381,0.003217061,0.000008628119,0.000018027844,0.000027380755,0.000012612472,0.99139166,0.00019581463,0.0011297148,0.0002637284,0.0036710831],"study_design_scores_gemma":[0.0000024073347,0.0000020821253,0.00020302224,0.0000010179007,6.0656834e-7,7.8751236e-7,0.0000015051129,0.99893004,0.00005731942,0.0007791435,0.000021179625,9.0675144e-7],"about_ca_topic_score_codex":0.030009115,"about_ca_topic_score_gemma":0.027080977,"teacher_disagreement_score":0.030009115,"about_ca_system_score_codex":0.0013991158,"about_ca_system_score_gemma":0.0006839467,"threshold_uncertainty_score":0.0596689},"labels":[],"label_agreement":null},{"id":"W4403198417","doi":"10.3847/1538-4357/ad684f","title":"IllustrisTNG in the HSC-SSP: No Shortage of Thin Disk Galaxies in TNG50","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Office of Science; Gauss Centre for Supercomputing; Toray Science Foundation; Ohio State University; High Energy Accelerator Research Organization; New Mexico State University; National Astronomical Observatory of Japan; Nuclear Safety and Security Commission; Japan Science and Technology Agency; U.S. Department of Energy; National Natural Science Foundation of China; York University; Carnegie Mellon University; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ministry of Education, Culture, Sports, Science and Technology; Harvard University; Brookhaven National Laboratory; Cabinet Office, Government of Japan; University of Portsmouth; Yale University; Vanderbilt University; National Science Foundation; National Aeronautics and Space Administration; Academia Sinica","keywords":"Physics; Galaxy; Economic shortage; Stars; Astrophysics; Astronomy","score_opus":0.007763944446503169,"score_gpt":0.22200450944200906,"score_spread":0.2142405649955059,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403198417","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9913065,0.00005082341,0.00245932,0.00020370646,0.000011515304,0.000008888313,0.000686176,0.00036443208,0.004908628],"genre_scores_gemma":[0.99658006,0.000019106488,0.0016954715,0.000083408515,0.0000038624057,0.000007719777,0.0010124316,0.00008567197,0.0005122887],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998785,0.000027551438,0.0000034824077,0.000039196148,0.000023899353,0.000027242297],"domain_scores_gemma":[0.9995975,0.00007068643,0.000051967636,0.00011579199,0.000049989805,0.0001140949],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003248159,0.00022590066,0.0002420606,0.0002415131,0.00040366143,0.00072107813,0.0006359712,0.00043572715,0.0029281196],"category_scores_gemma":[0.0015515817,0.00021328659,0.0003431519,0.00032246477,0.00041377696,0.00042576506,0.0005591244,0.00035400715,0.00047154396],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005617125,0.00021911637,0.43574527,0.00010960793,0.00023638448,0.0010838252,0.00078536564,0.48794246,0.020856775,0.018240085,0.012639459,0.021580005],"study_design_scores_gemma":[0.00014647857,0.00016570676,0.19905764,0.00003693756,0.00007397674,0.00034321554,0.0005378267,0.776216,0.008925793,0.006795662,0.0076511223,0.000049652328],"about_ca_topic_score_codex":0.018248932,"about_ca_topic_score_gemma":0.013850739,"teacher_disagreement_score":0.018248932,"about_ca_system_score_codex":0.0008925263,"about_ca_system_score_gemma":0.0003773997,"threshold_uncertainty_score":0.03628546},"labels":[],"label_agreement":null},{"id":"W4403225836","doi":"10.3847/1538-4357/ad6771","title":"AGN STORM 2. IX. Studying the Dynamics of the Ionized Obscurer in Mrk 817 with High-resolution X-Ray Spectroscopy","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council; Astrophysics Science Division; University of California, Irvine; Alexander von Humboldt-Stiftung; National Aeronautics and Space Administration; Chinese Academy of Sciences; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Outflow; Galaxy; Ionization; Astronomy; Accretion (finance); Spectral line; Active galactic nucleus; Line-of-sight; Emission spectrum; Absorption (acoustics); Line (geometry); Absorption spectroscopy; Optics","score_opus":0.010036945046338742,"score_gpt":0.22703158370525298,"score_spread":0.21699463865891425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403225836","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992107,0.00003090245,0.000100514575,0.000011834224,0.0000014152416,0.000002971039,0.00013328073,0.000012781821,0.0004955289],"genre_scores_gemma":[0.9977895,0.00003400821,0.00059549906,0.000020305584,0.00000969332,0.0000054851257,0.0008290507,0.000011928242,0.00070458895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993694,0.00000439055,0.0000032413895,0.000013304532,0.000020368276,0.000021762478],"domain_scores_gemma":[0.99982125,0.000011588712,0.0000754467,0.000016740298,0.000024040322,0.00005095757],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015385171,0.00015757413,0.00024328666,0.00044445446,0.00037911773,0.00039754607,0.00020165723,0.00022108687,0.0007036015],"category_scores_gemma":[0.00015958321,0.0000893905,0.0001968009,0.00022242292,0.00010716251,0.00020707991,0.00034405998,0.0002535675,0.00046929962],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003226522,0.00016829974,0.7525023,0.000046051457,0.00006210112,0.002732844,0.0006107781,0.0010509219,0.22729631,0.00032191345,0.0008403031,0.014045375],"study_design_scores_gemma":[0.0000065196705,0.0001170422,0.9925195,0.000002801034,0.000009068126,0.00037381274,0.00012929247,0.0012095708,0.004647503,0.000039919963,0.000939944,0.000004994907],"about_ca_topic_score_codex":0.0023623619,"about_ca_topic_score_gemma":0.0050492454,"teacher_disagreement_score":0.0023623619,"about_ca_system_score_codex":0.00022858207,"about_ca_system_score_gemma":0.00011790222,"threshold_uncertainty_score":0.0046972632},"labels":[],"label_agreement":null},{"id":"W4403254627","doi":"10.3847/1538-4357/ad6c08","title":"Multistructured Accretion Flow of Sgr A*. I. Examination of a Radiatively Inefficient Accretion Flow Model","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Fondo Nacional de Desarrollo Científico y Tecnológico; National Aeronautics and Space Administration; Agencia Nacional de Investigación y Desarrollo; Canada Research Chairs; Deutsche Forschungsgemeinschaft; Smithsonian Institution","keywords":"Physics; Accretion (finance); Astrophysics; Flow (mathematics); Accretion disc; Astronomy; Mechanics","score_opus":0.014281685740586877,"score_gpt":0.24325513872656832,"score_spread":0.22897345298598143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403254627","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9355255,0.00076261803,0.03833339,0.001809411,0.00011307125,0.00012241772,0.000531907,0.00030175777,0.022499904],"genre_scores_gemma":[0.9944689,0.0001644141,0.002382988,0.00012504627,0.00006840459,0.000029543624,0.0001186291,0.000042636682,0.0025993346],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984324,0.000048413338,0.000010072078,0.00003617788,0.000022307831,0.000039679857],"domain_scores_gemma":[0.9993704,0.00012558243,0.00021692883,0.000065757544,0.00005624262,0.0001650997],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00063954724,0.00068540673,0.0007937778,0.0006349143,0.00075052923,0.0015070818,0.0014256116,0.0010852469,0.0019533844],"category_scores_gemma":[0.0014881266,0.00035133527,0.0011012832,0.00021225215,0.0011828538,0.0012987717,0.00087998895,0.00058491743,0.0004457495],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039704936,0.00030978757,0.03437618,0.00015150328,0.00014985206,0.0017361813,0.00053713116,0.75948954,0.013546854,0.176954,0.003552679,0.00879919],"study_design_scores_gemma":[0.00004608599,0.000051845083,0.004194997,0.000011338795,0.000012430686,0.0001325472,0.000045871828,0.98302543,0.00023194638,0.011725754,0.00050037773,0.000021400256],"about_ca_topic_score_codex":0.013777523,"about_ca_topic_score_gemma":0.003446089,"teacher_disagreement_score":0.013777523,"about_ca_system_score_codex":0.0015705976,"about_ca_system_score_gemma":0.0006776681,"threshold_uncertainty_score":0.027394652},"labels":[],"label_agreement":null},{"id":"W4403254731","doi":"10.3847/1538-4357/ad6866","title":"Multistructured Accretion Flow of Sgr A*. II. Signatures of a Cool Accretion Disk in Hydrodynamic Simulations of Stellar Winds","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Ames Research Center; Fondo Nacional de Desarrollo Científico y Tecnológico; National Aeronautics and Space Administration; Agencia Nacional de Investigación y Desarrollo; Canada Research Chairs; Deutsche Forschungsgemeinschaft; Smithsonian Institution","keywords":"Physics; Astrophysics; Accretion (finance); Supermassive black hole; Stars; Spectral line; Astronomy; Galactic Center; Plasma; Galaxy","score_opus":0.007358438622540188,"score_gpt":0.24137681240067507,"score_spread":0.2340183737781349,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403254731","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965448,0.00003383527,0.0012312139,0.00011111597,0.000012239386,0.000014147574,0.00017058114,0.00007270434,0.0018094177],"genre_scores_gemma":[0.9986406,0.000017452818,0.00088803255,0.000026775859,0.0000041115013,0.000008496404,0.00016360333,0.000014212389,0.00023670064],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991155,0.000026190783,0.000006014356,0.000015507612,0.000015418515,0.000025395],"domain_scores_gemma":[0.99950147,0.00019717953,0.00008790001,0.000054515724,0.000062998144,0.000095895855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003489263,0.00028066713,0.0003350456,0.00028590774,0.00034757686,0.00074847223,0.0005720791,0.000525546,0.0009019021],"category_scores_gemma":[0.0013863193,0.00018334089,0.00046654488,0.0001817332,0.00057379,0.0003876309,0.0003783752,0.00051639037,0.0001255927],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028260835,0.00018815526,0.034799512,0.000031785406,0.00009239612,0.00025265053,0.00013195307,0.9539968,0.0048074704,0.002434649,0.00053490046,0.0024471972],"study_design_scores_gemma":[0.000047940932,0.00004766544,0.0051912274,0.0000035483363,0.000008284852,0.000013952963,0.000044839544,0.99362373,0.0005290387,0.00033097988,0.00015346482,0.000005383452],"about_ca_topic_score_codex":0.014084126,"about_ca_topic_score_gemma":0.0055789812,"teacher_disagreement_score":0.014084126,"about_ca_system_score_codex":0.0007084899,"about_ca_system_score_gemma":0.0005262423,"threshold_uncertainty_score":0.028004289},"labels":[],"label_agreement":null},{"id":"W4403255150","doi":"10.3847/1538-4357/ad6a18","title":"UNCOVER NIRSpec/PRISM Spectroscopy Unveils Evidence of Early Core Formation in a Massive, Centrally Dusty Quiescent Galaxy at z <sub>spec</sub> = 3.97","year":2024,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Institut National de Physique Nucléaire et de Physique des Particules; Center for Interdisciplinary Exploration and Research in Astrophysics, Northwestern University; Centre National de la Recherche Scientifique; National Research Foundation; Brinson Foundation; University of Toronto; Centre National d’Etudes Spatiales; Rijksuniversiteit Groningen; European Commission; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics","score_opus":0.019954533459644756,"score_gpt":0.26141990537409876,"score_spread":0.241465371914454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403255150","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9667057,0.00037580347,0.006153636,0.0006020941,0.00006725844,0.00002368729,0.0027741292,0.0020535986,0.021244047],"genre_scores_gemma":[0.9924826,0.00006371526,0.0035029445,0.00026851156,0.000036302026,0.000005366767,0.0017520604,0.00016283532,0.0017255429],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99982566,0.000009407528,0.0000061191677,0.0000444108,0.000057110257,0.000057342473],"domain_scores_gemma":[0.99946696,0.00004900609,0.00011528514,0.000120464465,0.00007316538,0.00017504006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036565744,0.0003117747,0.00025868823,0.00079699414,0.0003391561,0.0008264116,0.00050814514,0.00043492392,0.0047108377],"category_scores_gemma":[0.0004550684,0.00035864394,0.0003895528,0.00044709866,0.00035003677,0.00048659407,0.0008272711,0.0007507281,0.0022749698],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000986565,0.00027034318,0.32187647,0.00016646173,0.00017346778,0.0027160777,0.00060417515,0.002178003,0.6121929,0.0031174347,0.012268761,0.043449298],"study_design_scores_gemma":[0.00005768386,0.00021830243,0.931765,0.00002468573,0.00009505519,0.0016739377,0.00028250623,0.011334571,0.040391307,0.0019811543,0.012131187,0.000044579607],"about_ca_topic_score_codex":0.0022062652,"about_ca_topic_score_gemma":0.004060398,"teacher_disagreement_score":0.0047108377,"about_ca_system_score_codex":0.0003734731,"about_ca_system_score_gemma":0.00023672981,"threshold_uncertainty_score":0.01575929},"labels":[],"label_agreement":null},{"id":"W4403256011","doi":"10.3847/1538-4357/ad6b1e","title":"Simulation-based Inference of Radio Millisecond Pulsars in Globular Clusters","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"HORIZON EUROPE Framework Programme; Goddard Space Flight Center; Centre National de la Recherche Scientifique; Centre National d’Etudes Spatiales; Institut National de Physique Nucléaire et de Physique des Particules; National Aeronautics and Space Administration; Canada Research Chairs; Agence Nationale de la Recherche; Natural Sciences and Engineering Research Council of Canada; European Commission","keywords":"Globular cluster; Physics; Millisecond pulsar; Population; Luminosity; Astrophysics; Luminosity function; Algorithm; Pulsar; Computer science; Stars; Galaxy","score_opus":0.008643143794162712,"score_gpt":0.2414612918910222,"score_spread":0.2328181480968595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403256011","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8764306,0.00028500962,0.11846853,0.0006777857,0.00006315088,0.00007166538,0.0005264489,0.0007247714,0.0027522196],"genre_scores_gemma":[0.97285044,0.000093818635,0.025482006,0.00011234286,0.000036090987,0.00006202428,0.0006341609,0.00007605319,0.00065313047],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99962354,0.00018464113,0.000019598298,0.00007117193,0.00004293205,0.000058166446],"domain_scores_gemma":[0.98768693,0.010539661,0.00051529,0.000320939,0.0005104571,0.00042683308],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0027624536,0.0004523624,0.0008019017,0.001029494,0.0006786534,0.0012141567,0.0016031791,0.0011584796,0.0023654555],"category_scores_gemma":[0.014743471,0.0006108816,0.0008654015,0.00060095405,0.0010784961,0.0009939517,0.0011799544,0.0012725034,0.0002412075],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005737725,0.000024941146,0.010750574,0.000013798106,0.000036317026,0.000039389703,0.00003864644,0.98353255,0.00018031726,0.0028592357,0.00024109753,0.0022258908],"study_design_scores_gemma":[0.0000068929994,0.000004270127,0.00053087255,0.0000025871168,0.0000030608685,0.0000032994121,0.0000058729092,0.99834764,0.00005524593,0.0009925129,0.00004511343,0.000002598573],"about_ca_topic_score_codex":0.02844787,"about_ca_topic_score_gemma":0.020665884,"teacher_disagreement_score":0.02844787,"about_ca_system_score_codex":0.001318911,"about_ca_system_score_gemma":0.0014081729,"threshold_uncertainty_score":0.05656457},"labels":[],"label_agreement":null},{"id":"W4403280931","doi":"10.3847/1538-4357/ad6a13","title":"Contemporaneous X-Ray Observations of 30 Bright Radio Bursts from the Prolific Fast Radio Burst Source FRB 20220912A","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Simon Fraser University; Perimeter Institute; York University; University of British Columbia; McGill University; Canadian Institute for Theoretical Astrophysics; Ontario Power Generation; University of Toronto","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; University of Toronto; Smithsonian Astrophysical Observatory; McGill University; Canadian Institute for Advanced Research; Canada Research Chairs; University of Leicester; Canada Foundation for Innovation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Fast radio burst; Astrophysics; Astronomy; Gamma-ray burst; Neutron star","score_opus":0.01794898958142561,"score_gpt":0.2817603238518381,"score_spread":0.2638113342704125,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403280931","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982456,0.000052180883,0.00019244767,0.000017985054,0.0000038631533,0.000007776333,0.000605759,0.00002595552,0.00084848626],"genre_scores_gemma":[0.99492973,0.000047630696,0.0008176886,0.000024328048,0.000020036035,0.000014840086,0.0036429663,0.000017122684,0.0004856498],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998098,0.000018244282,0.000009794486,0.000049906426,0.00006667183,0.00004567581],"domain_scores_gemma":[0.9994067,0.000054532655,0.00016812288,0.00007590232,0.00011250397,0.00018232275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003253493,0.00028823357,0.00038611898,0.0012751021,0.0006344987,0.00038258813,0.00031880307,0.0003598512,0.0011314243],"category_scores_gemma":[0.0005597421,0.00022497188,0.00027006946,0.00067662494,0.00017936679,0.00014822198,0.0005706504,0.0003447005,0.00057303766],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010473512,0.0003362269,0.8504936,0.00007681692,0.00015979515,0.0012997319,0.00060344517,0.0011953834,0.11284766,0.0002139258,0.0013147931,0.030411275],"study_design_scores_gemma":[0.000009502204,0.000079629215,0.99749786,0.0000041602493,0.000013830267,0.00022636904,0.000037278955,0.0003315164,0.0009572229,0.000017533219,0.0008184981,0.0000066113003],"about_ca_topic_score_codex":0.008665616,"about_ca_topic_score_gemma":0.02239794,"teacher_disagreement_score":0.008665616,"about_ca_system_score_codex":0.00036798575,"about_ca_system_score_gemma":0.00022133513,"threshold_uncertainty_score":0.017230392},"labels":[],"label_agreement":null},{"id":"W4403311334","doi":"10.3847/1538-4357/ad738c","title":"The Anisotropic Circumgalactic Medium of Sub-L* Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Brookhaven National Laboratory; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; Fundamental Research Funds for the Central Universities; National Key Research and Development Program of China; Science and Technology Facilities Council; Ministerio de Ciencia e Innovación; Vanderbilt University; Consejo Nacional de Ciencia y Tecnología; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; U.S. Department of Energy; National Natural Science Foundation of China; Deutsche Forschungsgemeinschaft; York University; Huazhong University of Science and Technology; Carnegie Mellon University; Office of Science; Alfred P. Sloan Foundation; University of Washington; Princeton University; Johns Hopkins University; College of Engineering, Michigan State University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Gordon and Betty Moore Foundation; National Science Foundation","keywords":"Physics; Galaxy; Astrophysics; Anisotropy; Intergalactic medium; Astronomy; Quasar; Redshift; Optics","score_opus":0.006884918990453554,"score_gpt":0.2161748475837927,"score_spread":0.20928992859333917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403311334","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989672,0.000051850788,0.00019152921,0.000009669156,5.9692695e-7,0.0000010759883,0.00007285411,0.000008823821,0.0006963915],"genre_scores_gemma":[0.9998122,0.000022032731,0.00005395433,0.000004022949,0.0000014596538,3.7783585e-7,0.000058444846,0.0000014008026,0.00004606674],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999448,0.0000073422375,0.0000023434525,0.000018047447,0.000010717874,0.000016647095],"domain_scores_gemma":[0.9996736,0.00005709586,0.00012831336,0.000030765088,0.000028303582,0.000081829414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00008528548,0.00014262565,0.000117027754,0.00080446457,0.00021368025,0.001226132,0.00015712313,0.000107078944,0.0008373297],"category_scores_gemma":[0.0004304853,0.00015886099,0.00006561051,0.00041929263,0.00033717856,0.00037294833,0.0005344414,0.00013902308,0.00018428346],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020195953,0.000022108,0.86496687,0.000026160627,0.00005886012,0.00033561373,0.0006135896,0.0013501811,0.123969674,0.001216018,0.00015909916,0.0070798565],"study_design_scores_gemma":[0.000004144966,0.00001632358,0.9939831,0.0000030195324,0.000012686655,0.00011896565,0.00030211112,0.0016834247,0.0032307717,0.00021747676,0.0004230424,0.000004867995],"about_ca_topic_score_codex":0.007696834,"about_ca_topic_score_gemma":0.007221812,"teacher_disagreement_score":0.007696834,"about_ca_system_score_codex":0.00034618,"about_ca_system_score_gemma":0.000084166495,"threshold_uncertainty_score":0.015304089},"labels":[],"label_agreement":null},{"id":"W4403396169","doi":"10.3847/1538-4357/ad6869","title":"Anomaly Detection and Approximate Similarity Searches of Transients in Real-time Data Streams","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Deutsches Elektronen-Synchrotron; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Science Mission Directorate; Pacific Northwest National Laboratory; Smithsonian Astrophysical Observatory; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Stockholms Universitet; Nuclear Safety and Security Commission; Queen's University; Gordon and Betty Moore Foundation; Queen's University Belfast; Los Alamos National Laboratory; University of Washington; Brinson Foundation; Alfred P. Sloan Foundation; Johns Hopkins University; Weizmann Institute of Science; University of Warwick; National Central University; Villum Fonden; Durham University; Northwestern University; Space Telescope Science Institute; National Aeronautics and Space Administration; Battelle; Trinity College Dublin; U.S. Department of Energy; Smithsonian Institution; European Commission; Directorate for Computer and Information Science and Engineering; California Institute of Technology; University of California, Santa Cruz; Heising-Simons Foundation; David and Lucile Packard Foundation; National Centre for Supercomputing Applications; Laboratory Directed Research and Development; National Science Foundation","keywords":"Galaxy; Physics; Anomaly detection; Supernova; Light curve; Astrophysics; Astronomy; Computer science; Data mining","score_opus":0.025957988558237787,"score_gpt":0.26620793582722274,"score_spread":0.24024994726898496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403396169","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.45765945,0.0006722173,0.50604266,0.0005944337,0.00013627844,0.00026902606,0.005817556,0.027002981,0.0018054786],"genre_scores_gemma":[0.82491404,0.00010183879,0.16610123,0.00009641985,0.00009445434,0.00013558984,0.0076458063,0.0002777632,0.0006326846],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99708444,0.00034108214,0.00032604983,0.0008080574,0.001188365,0.00025202075],"domain_scores_gemma":[0.99441105,0.0020020867,0.0009968707,0.0012868922,0.0009758233,0.00032730715],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002099706,0.00071256654,0.0008428367,0.003554012,0.00053453486,0.0019011562,0.0017725553,0.0008850321,0.0013646765],"category_scores_gemma":[0.013866726,0.00029895752,0.0006576185,0.003081995,0.0005244404,0.0021319888,0.001719866,0.00077282795,0.0010806127],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023184645,0.0007106259,0.2214053,0.00043043005,0.00036245032,0.0017397474,0.0010460373,0.13036655,0.046799023,0.008559524,0.013880334,0.57238156],"study_design_scores_gemma":[0.000046365305,0.00014908511,0.01374916,0.000014673506,0.000025651669,0.00039436787,0.00018664007,0.9680989,0.007971106,0.006166925,0.003172674,0.000024457393],"about_ca_topic_score_codex":0.003221737,"about_ca_topic_score_gemma":0.0034246629,"teacher_disagreement_score":0.003554012,"about_ca_system_score_codex":0.0006507967,"about_ca_system_score_gemma":0.0012028997,"threshold_uncertainty_score":0.0111044645},"labels":[],"label_agreement":null},{"id":"W4403434084","doi":"10.3847/1538-4357/ad6d62","title":"Gradient Technique Theory: Tracing Magnetic Field and Obtaining Magnetic Field Strength","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Laboratory Directed Research and Development; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Magnetic field; Computational physics; Field strength; Turbulence; Field (mathematics); Mach number; Magnetohydrodynamics; Field line; Mechanics; Classical mechanics; Astrophysics; Quantum mechanics","score_opus":0.0041003569149206005,"score_gpt":0.21800093614891985,"score_spread":0.21390057923399924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403434084","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.023186347,0.00026925246,0.9724701,0.00021429184,0.000036701033,0.00003344377,0.00006350896,0.00036739782,0.003358879],"genre_scores_gemma":[0.66137516,0.00059332815,0.33347145,0.00018199916,0.000110748275,0.000097556775,0.00009443037,0.00021222532,0.003863116],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99979466,0.00007947344,0.000006398491,0.000035966936,0.00006059221,0.000022910273],"domain_scores_gemma":[0.9996419,0.00016451704,0.00006691529,0.000044217086,0.000054131026,0.000028281613],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004394251,0.00045259143,0.00033365106,0.0011144578,0.00025401832,0.00065578567,0.000728681,0.0004756901,0.0013709408],"category_scores_gemma":[0.0018930933,0.00021582139,0.00018859288,0.00062541344,0.0009475274,0.0011891507,0.0008400316,0.0006554136,0.0003357316],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026863458,0.000071091876,0.0051643206,0.00025638303,0.00006638687,0.00046118087,0.00043359087,0.07550924,0.16942467,0.58151364,0.0026708748,0.16415998],"study_design_scores_gemma":[0.00003403551,0.00014668741,0.0033703693,0.00002802153,0.00002082437,0.0005451855,0.00007105133,0.766584,0.0423166,0.18065925,0.006162351,0.000061584404],"about_ca_topic_score_codex":0.0010006436,"about_ca_topic_score_gemma":0.00066721364,"teacher_disagreement_score":0.0013709408,"about_ca_system_score_codex":0.00033439684,"about_ca_system_score_gemma":0.0003623033,"threshold_uncertainty_score":0.00458622},"labels":[],"label_agreement":null},{"id":"W4403490514","doi":"10.3847/1538-4357/ad59aa","title":"Morphologies of Bright Complex Fast Radio Bursts with CHIME/FRB Voltage Data","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Canada Foundation for Innovation","keywords":"Physics; Astronomy; Astrophysics; Fast radio burst; Neutron star","score_opus":0.03233476849142999,"score_gpt":0.335641534974652,"score_spread":0.303306766483222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403490514","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879147,0.00066365715,0.0047202446,0.000088430075,0.000022721619,0.000039570146,0.0019913549,0.00040502325,0.0041543418],"genre_scores_gemma":[0.9904157,0.00017327451,0.0044715023,0.000043994878,0.000026522883,0.000023934637,0.0034203308,0.00011078574,0.0013139506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983025,0.00000824767,0.000008022608,0.00004695915,0.00007001939,0.000036546684],"domain_scores_gemma":[0.99935085,0.00010228271,0.0001936575,0.000095415475,0.0001318724,0.00012583652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019058025,0.00022403411,0.00022415377,0.0016031082,0.0003427127,0.00071988313,0.00038389242,0.00031422908,0.0018707311],"category_scores_gemma":[0.00111761,0.0001767379,0.00015611688,0.0016654514,0.0002585728,0.00021684014,0.00050264347,0.00023884006,0.0005452847],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008442417,0.00011167519,0.49849406,0.000321464,0.00017974342,0.004363047,0.0016919522,0.003382622,0.36385435,0.0015174571,0.0058653206,0.119374074],"study_design_scores_gemma":[0.000014558332,0.000055561704,0.97866756,0.000022417722,0.000030422081,0.0015395123,0.00019101678,0.0034745827,0.009013391,0.00025859982,0.0067052883,0.000027218655],"about_ca_topic_score_codex":0.007489713,"about_ca_topic_score_gemma":0.008698978,"teacher_disagreement_score":0.007489713,"about_ca_system_score_codex":0.0003961979,"about_ca_system_score_gemma":0.00015736932,"threshold_uncertainty_score":0.0148922205},"labels":[],"label_agreement":null},{"id":"W4403542238","doi":"10.3847/1538-4357/ad5f1e","title":"A More Precise Measurement of the Radius of PSR J0740+6620 Using Updated NICER Data","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":105,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Aeronautics and Space Administration","keywords":"RADIUS; Physics; Neutron star; Astrophysics; Computer science","score_opus":0.05723267630373662,"score_gpt":0.3650940605186162,"score_spread":0.3078613842148796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403542238","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96886116,0.0004610084,0.0063823983,0.00025161804,0.00006891343,0.000052566007,0.011350008,0.0016465775,0.010925731],"genre_scores_gemma":[0.960203,0.00021385305,0.011313328,0.00024312075,0.00008343572,0.0000734191,0.025430992,0.000589323,0.0018494878],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995035,0.00007119202,0.000039640694,0.00013931679,0.00016428936,0.0000820571],"domain_scores_gemma":[0.9986815,0.00010227359,0.00037914072,0.0003296703,0.0003184238,0.00018887245],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010986447,0.0004461933,0.00043235565,0.0017703596,0.0004047719,0.0007277483,0.00055371335,0.00048150079,0.002012558],"category_scores_gemma":[0.0015124341,0.0003638354,0.00063615694,0.0015135566,0.00019723822,0.00065240666,0.00086988654,0.0006392429,0.001622481],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00053673115,0.00014602706,0.8273199,0.00018621513,0.00039855027,0.0004604761,0.0006901347,0.0048210677,0.11866394,0.0007921902,0.010427473,0.035557278],"study_design_scores_gemma":[0.000034849345,0.00008071012,0.96680605,0.000025356754,0.000098648765,0.00023147654,0.00009887197,0.005647383,0.010964006,0.00014226597,0.015823131,0.000047215424],"about_ca_topic_score_codex":0.010853802,"about_ca_topic_score_gemma":0.024033865,"teacher_disagreement_score":0.010853802,"about_ca_system_score_codex":0.00062508305,"about_ca_system_score_gemma":0.00032313258,"threshold_uncertainty_score":0.021581233},"labels":[],"label_agreement":null},{"id":"W4403542247","doi":"10.3847/1538-4357/ad5f1f","title":"The Radius of the High-mass Pulsar PSR J0740+6620 with 3.6 yr of NICER Data","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":154,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Astrophysics Division; HORIZON EUROPE European Research Council; Astrophysics Science Division; Office of Naval Research; Smithsonian Institution; Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; Goddard Space Flight Center; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Smithsonian Astrophysical Observatory; Centre National d’Etudes Spatiales; National Aeronautics and Space Administration","keywords":"Algorithm; Physics; RADIUS; Computer science","score_opus":0.013746523952194428,"score_gpt":0.3108710029080735,"score_spread":0.29712447895587907,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403542247","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96657914,0.00070030504,0.0025728005,0.0002812877,0.00005148975,0.00002335156,0.019673858,0.00082299893,0.009294794],"genre_scores_gemma":[0.93413293,0.0003192658,0.0036829226,0.00021979658,0.00008697099,0.000049093975,0.058808617,0.0004811421,0.0022193303],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993575,0.00009218108,0.000035983587,0.00020035553,0.00021111651,0.00010281601],"domain_scores_gemma":[0.9986284,0.00015225694,0.00053262274,0.00033592733,0.0002245247,0.0001263391],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012318904,0.00039660808,0.00043428116,0.0015194968,0.00039507658,0.0009989543,0.00052581483,0.00039630328,0.0014193335],"category_scores_gemma":[0.0026616873,0.00038453192,0.00089323585,0.0014844503,0.0003633394,0.00066723494,0.0016008127,0.00048095535,0.0017032382],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005799049,0.000057593275,0.922894,0.00017594303,0.0004875347,0.0004557331,0.00037443952,0.014768964,0.016414734,0.0009184121,0.01353275,0.029340027],"study_design_scores_gemma":[0.00004686163,0.00008681738,0.94090503,0.000049355564,0.00014247795,0.0003957204,0.000118844575,0.012100305,0.0035166708,0.00034773283,0.04222876,0.00006132788],"about_ca_topic_score_codex":0.014889695,"about_ca_topic_score_gemma":0.022987397,"teacher_disagreement_score":0.014889695,"about_ca_system_score_codex":0.0007342964,"about_ca_system_score_gemma":0.0005111987,"threshold_uncertainty_score":0.029606044},"labels":[],"label_agreement":null},{"id":"W4403573075","doi":"10.3847/1538-4357/ad90b7","title":"Revisiting the Chemical Composition of WD 1145+017: Impact of Circumstellar Disk Contamination on Photospheric Abundances","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université du Québec","funders":"Natural Sciences and Engineering Research Council of Canada; Agencia Nacional de Investigación y Desarrollo; National Science Foundation; Korea Astronomy and Space Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Macquarie University; Space Telescope Science Institute","keywords":"Contamination; Composition (language); Abundance (ecology); Astrophysics; Chemical composition; Circumstellar disk; Physics; Astrobiology; Astronomy; Environmental science; Stars; Art; Biology; Ecology; Literature","score_opus":0.010744595767198934,"score_gpt":0.2586726086717603,"score_spread":0.24792801290456135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403573075","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977423,0.00020510133,0.0007251888,0.000049898783,0.000010161868,0.0000041036596,0.0005917958,0.000030515259,0.000640971],"genre_scores_gemma":[0.9985513,0.000047996295,0.00038981307,0.0000136237695,0.0000051832094,0.000001966604,0.0008041237,0.000016306185,0.00016959348],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998455,0.000023492332,0.000013047364,0.00004746007,0.000042915133,0.000027616921],"domain_scores_gemma":[0.99971145,0.000053828226,0.000073339295,0.000034153818,0.00008390601,0.000043379096],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00043184782,0.00031484652,0.00024867995,0.0012263148,0.00037838568,0.00074377836,0.000352203,0.00027794007,0.00092071394],"category_scores_gemma":[0.00068218977,0.00012423412,0.0003916087,0.0005914459,0.00021564902,0.0003911311,0.0004532302,0.00017620299,0.0002489931],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006749901,0.000018200148,0.96524173,0.000059491536,0.00012347405,0.00018794875,0.00013874077,0.0033131568,0.022992404,0.0003398243,0.0003823802,0.007135146],"study_design_scores_gemma":[0.000005703736,0.000035212342,0.9715574,0.000025735822,0.00009410586,0.00015397936,0.00029087169,0.014720459,0.008946098,0.00034244926,0.0038156116,0.000012409062],"about_ca_topic_score_codex":0.016407557,"about_ca_topic_score_gemma":0.017099425,"teacher_disagreement_score":0.016407557,"about_ca_system_score_codex":0.0007049741,"about_ca_system_score_gemma":0.00027770564,"threshold_uncertainty_score":0.032624066},"labels":[],"label_agreement":null},{"id":"W4403622363","doi":"10.3847/1538-4357/ad77a1","title":"Abundant Molecular Gas in the Central Region of Lenticular Galaxy PGC 39535","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; Centre National de la Recherche Scientifique; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Max-Planck-Gesellschaft; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Star formation; Spiral galaxy; Galaxy; Bulge; Star (game theory); Astronomy","score_opus":0.006422956818661133,"score_gpt":0.20908058529418122,"score_spread":0.20265762847552007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403622363","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99966395,0.000018942306,0.000028059385,0.0000032411413,2.712429e-7,7.658469e-7,0.00006931894,0.0000037411228,0.00021179862],"genre_scores_gemma":[0.99963593,0.0000112009375,0.00006834173,0.000004314534,7.1161065e-7,7.079432e-7,0.00019437152,6.8446417e-7,0.000083625186],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999578,0.0000023833384,0.0000020285854,0.000018066143,0.000009479691,0.000010127444],"domain_scores_gemma":[0.99988234,0.000008283857,0.000046756304,0.000011890796,0.000010324746,0.00004040968],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00005805223,0.00009963573,0.000085051666,0.0006298276,0.00026866517,0.00020185557,0.0001841598,0.00010997993,0.0006346959],"category_scores_gemma":[0.00011755399,0.000059572318,0.00009120958,0.00040652932,0.00025030415,0.00008841355,0.0002701879,0.000066966575,0.0000984944],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00010691617,0.00003420138,0.9262317,0.000023303706,0.000028294191,0.0005120051,0.000731981,0.00023890546,0.065670215,0.00019910878,0.00020732924,0.0060160635],"study_design_scores_gemma":[0.0000014321455,0.000016203892,0.9988612,0.0000016847928,0.0000044440308,0.000093832154,0.000115558265,0.00012441498,0.0005128341,0.000016469274,0.00025099795,0.0000010506348],"about_ca_topic_score_codex":0.014927651,"about_ca_topic_score_gemma":0.017740695,"teacher_disagreement_score":0.014927651,"about_ca_system_score_codex":0.00023699312,"about_ca_system_score_gemma":0.00008330652,"threshold_uncertainty_score":0.029681563},"labels":[],"label_agreement":null},{"id":"W4403651878","doi":"10.3847/1538-4357/ad7367","title":"On the Origin of Quenched but Gas-rich Regions at Kiloparsec Scales in Nearby Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Tsinghua University; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Galaxy; Astrophysics; Astronomy","score_opus":0.013265252357938854,"score_gpt":0.23115613733170653,"score_spread":0.21789088497376768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403651878","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99882454,0.00011078448,0.0003603655,0.000042732852,0.0000011978383,0.0000032727737,0.00012299958,0.00003355452,0.0005004897],"genre_scores_gemma":[0.99969923,0.00001555822,0.00014429973,0.000010475901,0.0000022847946,0.0000017446436,0.000059391186,0.000004941585,0.0000621374],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989736,0.000014814061,0.0000036298707,0.000040683983,0.000017510483,0.000026047781],"domain_scores_gemma":[0.9987457,0.00034185118,0.00040151758,0.00018122236,0.00008418786,0.00024552937],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003414345,0.00016262519,0.00021842484,0.00057806395,0.00031958206,0.0007071398,0.0005016692,0.00028201338,0.0012067828],"category_scores_gemma":[0.0013743155,0.00018605325,0.00021009272,0.00041067213,0.0006531193,0.00040184654,0.0004762636,0.00027271773,0.00027290866],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018411304,0.000049170587,0.9385935,0.000030593554,0.000055398395,0.0004655569,0.00069802505,0.0015329351,0.05083654,0.0012153143,0.00021181098,0.0061269877],"study_design_scores_gemma":[0.0000052968408,0.000023037122,0.9947765,0.0000043507134,0.000016229507,0.00010567527,0.00013376937,0.0021202827,0.002146949,0.0004098044,0.00025212872,0.000006032602],"about_ca_topic_score_codex":0.0049395575,"about_ca_topic_score_gemma":0.0055840835,"teacher_disagreement_score":0.0049395575,"about_ca_system_score_codex":0.00048533553,"about_ca_system_score_gemma":0.00010495111,"threshold_uncertainty_score":0.009821594},"labels":[],"label_agreement":null},{"id":"W4403661737","doi":"10.3847/1538-4357/adce70","title":"The Atacama Cosmology Telescope: Systematic Transient Search of Single Observation Maps","year":2025,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Institute of Standards and Technology; Agencia Nacional de Investigación y Desarrollo; University of Toronto; National Research Foundation; National Energy Research Scientific Computing Center; National Aeronautics and Space Administration; University of Pennsylvania; Princeton University; National Science Foundation; European Space Agency; Compute Canada; Simons Foundation; Government of Ontario","keywords":"Transient (computer programming); Cosmology; Physics; Telescope; Astronomy; Astrophysics; Computer science","score_opus":0.03222526641788531,"score_gpt":0.29175053680333923,"score_spread":0.2595252703854539,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403661737","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8797941,0.0009587927,0.0746578,0.00016467749,0.00004583307,0.00030267486,0.030937128,0.007805622,0.0053334427],"genre_scores_gemma":[0.8629111,0.00024596116,0.09193325,0.00007742287,0.00004664832,0.00018317893,0.042439245,0.0006436535,0.0015195346],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993944,0.00008086505,0.00004212623,0.0002073862,0.00017313726,0.000102027145],"domain_scores_gemma":[0.9969008,0.00037664137,0.0007029504,0.0009944475,0.0007073693,0.00031785906],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012698089,0.00037759184,0.00048695973,0.0044766646,0.0008002117,0.0010519505,0.0006312029,0.00033736666,0.0013420384],"category_scores_gemma":[0.0027523586,0.0003541646,0.00051074766,0.004461676,0.0002445595,0.0006399064,0.0010141323,0.00031870187,0.0009610485],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005968882,0.00017124896,0.66879344,0.00039342677,0.0006312235,0.0011905135,0.001182018,0.00677663,0.10391603,0.0014891847,0.019387038,0.19547229],"study_design_scores_gemma":[0.00005564457,0.000108336935,0.92612505,0.000041806186,0.0001539564,0.00054720655,0.0005031826,0.02966909,0.02186873,0.001357895,0.01951251,0.00005665403],"about_ca_topic_score_codex":0.012977947,"about_ca_topic_score_gemma":0.017905258,"teacher_disagreement_score":0.012977947,"about_ca_system_score_codex":0.0004197147,"about_ca_system_score_gemma":0.0014532552,"threshold_uncertainty_score":0.025804818},"labels":[],"label_agreement":null},{"id":"W4403690614","doi":"10.3847/1538-4357/ad778a","title":"Binary Yellow Supergiants in the Magellanic Clouds. I. Photometric Candidate Identification","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Space Telescope Science Institute","keywords":"Physics; Supergiant; Blue supergiant; Astronomy; Astrophysics; Large Magellanic Cloud; Photometry (optics); Binary star; Red supergiant; Stars","score_opus":0.011389376293880505,"score_gpt":0.24525102428502263,"score_spread":0.23386164799114212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403690614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99807125,0.00014652684,0.00069123413,0.0000099674935,0.0000011207463,0.000011536972,0.00042783824,0.000025865005,0.00061463163],"genre_scores_gemma":[0.99763143,0.00004713573,0.0011272631,0.000005817442,0.000001879354,0.0000067933825,0.0009686536,0.0000046096093,0.00020630377],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997739,0.00002953142,0.000012657641,0.000083093655,0.00005147955,0.000049299433],"domain_scores_gemma":[0.99916553,0.00018374117,0.0002605421,0.00013319022,0.000092184644,0.00016481969],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055072625,0.00032131645,0.00034431985,0.0024581451,0.00049111666,0.00077731116,0.00040453736,0.00022671542,0.0017499801],"category_scores_gemma":[0.00096442905,0.00015611867,0.00038058686,0.001254368,0.00028805225,0.00040003998,0.000954864,0.00020131988,0.00039640057],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011981159,0.000033816752,0.98393756,0.000017653967,0.000039138846,0.0000450074,0.00008595233,0.0016134433,0.005133564,0.0002067434,0.00014397067,0.008623342],"study_design_scores_gemma":[0.000010009513,0.00005371758,0.9847348,0.00000669935,0.00003750449,0.00013096734,0.0001526508,0.010816034,0.0031661822,0.0002616367,0.0006240427,0.0000058175433],"about_ca_topic_score_codex":0.008073249,"about_ca_topic_score_gemma":0.013785332,"teacher_disagreement_score":0.008073249,"about_ca_system_score_codex":0.00038045007,"about_ca_system_score_gemma":0.00029749266,"threshold_uncertainty_score":0.016052485},"labels":[],"label_agreement":null},{"id":"W4403750564","doi":"10.3847/1538-4357/ad779d","title":"Do All Fast Radio Bursts Repeat? Constraints from CHIME/FRB Far Sidelobe FRBs","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Fonds de recherche du Québec – Nature et technologies; McGill Space Institute; National Defense Science and Engineering Graduate; Smithsonian Astrophysical Observatory; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; Mitacs; National Research Council Canada; University of Toronto; Industry Canada; Government of Ontario; National Natural Science Foundation of China; Canada Foundation for Innovation; Canada Research Chairs; Ontario Centres of Excellence; Alexander von Humboldt-Stiftung; U.S. Department of Defense; McGill University; Canadian Institute for Advanced Research; Government of Canada; National Science Foundation","keywords":"Physics; Astronomy; Astrophysics; Fast radio burst; Radio astronomy; Galaxy","score_opus":0.014336245797723163,"score_gpt":0.31616753575379675,"score_spread":0.30183128995607356,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403750564","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99506396,0.00017047668,0.0015197609,0.00007810814,0.0000041478906,0.000011105138,0.0009094132,0.000102959195,0.0021401222],"genre_scores_gemma":[0.99835664,0.000030667677,0.00059639214,0.000024500521,0.0000054294633,0.000004527574,0.0007536496,0.000023484748,0.00020455816],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99950993,0.000041690404,0.000018777866,0.0001633552,0.00012498556,0.00014123374],"domain_scores_gemma":[0.99710494,0.00075123215,0.0007414996,0.00041543497,0.00037984768,0.00060706434],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00070060225,0.0003831756,0.0004120048,0.001111836,0.00066741975,0.000760568,0.0005438381,0.0005159048,0.0016543336],"category_scores_gemma":[0.0027553835,0.000385953,0.00030015927,0.00073132524,0.00052311586,0.00029272324,0.00054907106,0.00039589324,0.000476547],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030224104,0.00003306532,0.960104,0.00003967955,0.00009865533,0.0003800858,0.00035269823,0.0017695957,0.026279133,0.00030335973,0.00075733114,0.009580217],"study_design_scores_gemma":[0.000005576114,0.000017646815,0.99545825,0.0000054849543,0.000018446357,0.00015920684,0.00008467427,0.0019850493,0.0012583211,0.000097472956,0.0008987954,0.0000111047075],"about_ca_topic_score_codex":0.0695296,"about_ca_topic_score_gemma":0.14527982,"teacher_disagreement_score":0.0695296,"about_ca_system_score_codex":0.0009971091,"about_ca_system_score_gemma":0.00048092232,"threshold_uncertainty_score":0.13824975},"labels":[],"label_agreement":null},{"id":"W4403750668","doi":"10.3847/1538-4357/ad7735","title":"Modeling and Subtracting Diffuse Cluster Light in JWST Images: A Relation between the Spatial Distribution of Globular Clusters, Dwarf Galaxies, and Intracluster Light in the Lensing Cluster SMACS 0723","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Research Council; Alliance de recherche numérique du Canada; Javna Agencija za Raziskovalno Dejavnost RS; Canadian Space Agency; Space Telescope Science Institute; Canarie; Canadian Foundation for AIDS Research; National Aeronautics and Space Administration","keywords":"Physics; Globular cluster; Astrophysics; Astronomy; Galaxy cluster; Dark matter; Dwarf galaxy; Cluster (spacecraft); Galaxy; James Webb Space Telescope; Brightest cluster galaxy","score_opus":0.010247621922826545,"score_gpt":0.2256292216459181,"score_spread":0.21538159972309154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403750668","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9798522,0.000037239784,0.019295555,0.000035862264,0.0000026606983,0.000014091626,0.00021752197,0.000121280915,0.00042359956],"genre_scores_gemma":[0.98793644,0.000023485512,0.011308612,0.000011279891,0.0000051712395,0.000016882344,0.00042702068,0.000028039884,0.00024292164],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981815,0.000026947022,0.000008376812,0.000062950596,0.00005992512,0.000023717066],"domain_scores_gemma":[0.9995554,0.00014085614,0.00010846407,0.00007849311,0.0000653153,0.000051437484],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00050109834,0.00037925655,0.0002516967,0.001086187,0.00028410755,0.0007108475,0.0006792228,0.0003161402,0.00035477034],"category_scores_gemma":[0.001518302,0.00027203138,0.0004709063,0.00078611675,0.00026205787,0.00028118296,0.0003697408,0.00025813805,0.00016874283],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015946971,0.00015691952,0.6258136,0.000042634627,0.00030265725,0.00012893058,0.00025097126,0.30277526,0.03245619,0.0016499205,0.0005222093,0.035741165],"study_design_scores_gemma":[0.000012296585,0.000039432165,0.2816195,0.000006921184,0.000054385415,0.000057902307,0.00011067095,0.7099003,0.0069942465,0.0005319531,0.0006513084,0.000021066619],"about_ca_topic_score_codex":0.044459857,"about_ca_topic_score_gemma":0.04619976,"teacher_disagreement_score":0.044459857,"about_ca_system_score_codex":0.0009574399,"about_ca_system_score_gemma":0.0005746583,"threshold_uncertainty_score":0.08840215},"labels":[],"label_agreement":null},{"id":"W4403752401","doi":"10.3847/1538-4357/ad7bb4","title":"Kinematic Analysis of z = 4.3 Galaxies in the SPT2349–56 Protocluster Core","year":2024,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; Associated Universities; Max-Planck-Gesellschaft; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Core (optical fiber); Kinematics; Galaxy; Astrophysics; Physics; Classical mechanics; Optics","score_opus":0.029521799651564054,"score_gpt":0.32750725370644407,"score_spread":0.29798545405488003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403752401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99904567,0.000035213267,0.00009970752,0.000010895845,0.0000020360612,0.0000044743074,0.00042743052,0.000023341632,0.00035118256],"genre_scores_gemma":[0.9968375,0.000032775166,0.0003957593,0.000010091972,0.0000067730257,0.000006234191,0.0024154957,0.000011516647,0.0002839097],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982125,0.000011496916,0.0000090677695,0.00005786487,0.000054911736,0.000045382894],"domain_scores_gemma":[0.99936765,0.000051153507,0.00023506659,0.000062262334,0.00008045183,0.00020353816],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017559149,0.00029015477,0.0003081526,0.0023602669,0.0004076858,0.0005855799,0.0003812961,0.00018088109,0.0013095245],"category_scores_gemma":[0.00070645777,0.00018031095,0.00033724494,0.0013583493,0.00029017054,0.0001784235,0.0008214042,0.00020795307,0.0005233934],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015079863,0.000043420812,0.97230434,0.000022291704,0.00006144709,0.00056832517,0.0004055264,0.0005921864,0.016019277,0.0001277006,0.0006825749,0.009022091],"study_design_scores_gemma":[0.0000040427444,0.000019859406,0.9981117,0.0000035400199,0.000011229933,0.00018035824,0.00008952186,0.000596343,0.0006050375,0.00002192031,0.00035277862,0.000003786029],"about_ca_topic_score_codex":0.011119187,"about_ca_topic_score_gemma":0.011658592,"teacher_disagreement_score":0.011119187,"about_ca_system_score_codex":0.0004537658,"about_ca_system_score_gemma":0.00020350845,"threshold_uncertainty_score":0.022108912},"labels":[],"label_agreement":null},{"id":"W4403758235","doi":"10.3847/1538-4357/ad738f","title":"The Power of High-precision Broadband Photometry: Tracing the Milky Way Density Profile with Blue Horizontal Branch Stars in the Dark Energy Survey","year":2024,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Milky Way; Photometry (optics); Stars; Astronomy; Astrophysics; Broadband; Tracing; Optics","score_opus":0.009239943001605801,"score_gpt":0.22293185318738376,"score_spread":0.21369191018577796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403758235","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92938197,0.0004872994,0.06544485,0.00046973914,0.000010087511,0.00002505341,0.0012690169,0.00071623595,0.0021957436],"genre_scores_gemma":[0.97214985,0.00018421681,0.025230858,0.000060081187,0.000024876743,0.00001532866,0.0015096762,0.0000639902,0.0007611775],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99955314,0.00016123592,0.000019191102,0.00012075666,0.00010032995,0.00004536657],"domain_scores_gemma":[0.99816495,0.0006603103,0.0004474537,0.00039933805,0.00016883296,0.00015915389],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014397461,0.0003381011,0.0002454172,0.0012492714,0.00027077406,0.0014172676,0.00065222103,0.00068595435,0.00060988276],"category_scores_gemma":[0.004293929,0.00044866573,0.0005081749,0.0010900036,0.0003254383,0.0009558002,0.0009894067,0.0003784587,0.0004543802],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009389743,0.0000667539,0.85620826,0.000040982977,0.00016611694,0.000077743025,0.00015440492,0.08505925,0.0068193306,0.0024428905,0.0014672293,0.047403164],"study_design_scores_gemma":[0.00002724601,0.000054798576,0.4598153,0.000036109555,0.000072512725,0.00012552219,0.00012104851,0.5289798,0.0042763427,0.003742213,0.0026968676,0.000052242507],"about_ca_topic_score_codex":0.016130988,"about_ca_topic_score_gemma":0.025912957,"teacher_disagreement_score":0.016130988,"about_ca_system_score_codex":0.00049654307,"about_ca_system_score_gemma":0.00035307705,"threshold_uncertainty_score":0.032074153},"labels":[],"label_agreement":null},{"id":"W4403771943","doi":"10.3847/1538-4357/ad66cc","title":"To High Redshift and Low Mass: Exploring the Emergence of Quenched Galaxies and Their Environments at 3 &lt; z &lt; 6 in the Ultra-deep JADES MIRI F770W Parallel","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":39,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; Goddard Space Flight Center; Ministerio de Ciencia e Innovación; Nuclear Safety and Security Commission; European Commission; Science and Technology Facilities Council; National Research Foundation; UK Research and Innovation; Space Telescope Science Institute; University of California, Santa Cruz; Danmarks Grundforskningsfond; University of Arizona; Aspen Center for Physics; National Science Foundation; European Space Agency; National Aeronautics and Space Administration","keywords":"Physics; Redshift; Astrophysics; Galaxy; Red shift; Astronomy","score_opus":0.011498096768149188,"score_gpt":0.20493802176655465,"score_spread":0.19343992499840545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403771943","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99922585,0.000026104868,0.00008270429,0.000030286914,9.418132e-7,0.0000024817355,0.00022043163,0.000009872787,0.0004013302],"genre_scores_gemma":[0.9987853,0.000022043796,0.00021819552,0.000047751884,0.0000045638553,0.000004099442,0.0006080439,0.000011483756,0.00029863635],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984646,0.000014561494,0.0000038837593,0.000046897076,0.00003386714,0.00005429034],"domain_scores_gemma":[0.9994035,0.00004519742,0.00016421072,0.00004136354,0.000083886865,0.0002618623],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002915079,0.00015508881,0.00022921148,0.00086025614,0.0004969005,0.0007766796,0.00041715748,0.00023153736,0.00094978797],"category_scores_gemma":[0.0007202468,0.00015214687,0.00018758106,0.0004306714,0.00043437682,0.00040536618,0.00087520666,0.0003615187,0.0002814984],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014442265,0.00010982749,0.97831774,0.000010631084,0.000035502802,0.00024184768,0.0013275992,0.00022879799,0.011201885,0.0003021741,0.0006946138,0.007384866],"study_design_scores_gemma":[0.000001212478,0.000009773107,0.9992348,0.0000016401195,0.0000028611123,0.00002840633,0.00013996162,0.00014837013,0.00017563024,0.000020396761,0.00023523693,0.000001698885],"about_ca_topic_score_codex":0.014936039,"about_ca_topic_score_gemma":0.028051462,"teacher_disagreement_score":0.014936039,"about_ca_system_score_codex":0.0005097392,"about_ca_system_score_gemma":0.00018430436,"threshold_uncertainty_score":0.029698193},"labels":[],"label_agreement":null},{"id":"W4403776482","doi":"10.3847/1538-4357/ad7a6a","title":"Magnetic Field Evolution for Crystallization-driven Dynamos in C/O White Dwarfs","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Engineering and Physical Sciences Research Council; Natural Sciences and Engineering Research Council of Canada","keywords":"White dwarf; Physics; Dynamo; Astrophysics; Magnetic field; Astronomy; Crystallization; Field (mathematics); Dynamo theory; Stars","score_opus":0.007011213906140851,"score_gpt":0.22551554249678865,"score_spread":0.2185043285906478,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403776482","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99867755,0.000021483142,0.00064656057,0.000028581495,0.000002025154,0.0000029726527,0.000031236537,0.000032775595,0.0005567827],"genre_scores_gemma":[0.9995838,0.000008228434,0.00024049163,0.00000528936,0.0000011263995,0.000002353027,0.00003051344,0.0000072365206,0.000121057514],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999695,0.0000049086802,0.0000020085117,0.000006335938,0.0000070635597,0.0000102295235],"domain_scores_gemma":[0.9997743,0.000059926377,0.000057240366,0.000014404842,0.00004130346,0.000052789204],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016212849,0.00021199933,0.00023726354,0.0002957932,0.00030048253,0.00040327522,0.00022491332,0.0002444996,0.00069048285],"category_scores_gemma":[0.00065790344,0.00011162029,0.00023795996,0.00014628224,0.00040238068,0.0001798367,0.00021342431,0.00021829367,0.000078110665],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000909756,0.00026399188,0.1639484,0.00011435794,0.00011287289,0.0013466263,0.00034428423,0.48500222,0.32935038,0.0083501935,0.00076107396,0.009495874],"study_design_scores_gemma":[0.00011632456,0.00020860293,0.07857979,0.0000105756,0.000024040073,0.00015192636,0.00016975429,0.88253367,0.035407852,0.0021743765,0.0005910554,0.000031931377],"about_ca_topic_score_codex":0.0053541744,"about_ca_topic_score_gemma":0.0027012946,"teacher_disagreement_score":0.0053541744,"about_ca_system_score_codex":0.0008495758,"about_ca_system_score_gemma":0.00030462432,"threshold_uncertainty_score":0.010645986},"labels":[],"label_agreement":null},{"id":"W4403813970","doi":"10.3847/1538-4357/ad76a0","title":"Lower-mass-gap Black Holes in Dense Star Clusters","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Star (game theory); Star cluster; Stars","score_opus":0.015685849051945543,"score_gpt":0.2449915725532289,"score_spread":0.22930572350128337,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403813970","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99629056,0.000060996696,0.0025016635,0.000075204014,0.0000054635407,0.000007056417,0.000043813638,0.000020661373,0.0009945811],"genre_scores_gemma":[0.9994246,0.000019101399,0.00028461343,0.000007729057,0.0000033619583,0.000002240346,0.000025659017,0.000002761297,0.00023001047],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999075,0.000026229745,0.0000027942633,0.000020642834,0.000013462841,0.000029374549],"domain_scores_gemma":[0.9995552,0.00013575095,0.000106739695,0.000034804332,0.000029258032,0.0001381421],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00031986862,0.00025839242,0.0004485338,0.00031161302,0.00052948174,0.0010023654,0.0006384936,0.00045340566,0.0017635251],"category_scores_gemma":[0.0010220688,0.00023508898,0.00029088708,0.0002077848,0.00101997,0.000508693,0.000729341,0.00028336444,0.0001338072],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020253425,0.0001221788,0.12310958,0.000036066558,0.00007219956,0.0006162128,0.00025547584,0.8387583,0.0030413636,0.030427037,0.00072612526,0.0026328904],"study_design_scores_gemma":[0.000096748736,0.00007394385,0.034689717,0.00000834091,0.000020545553,0.00012406231,0.00013028231,0.9489122,0.0005864287,0.014705927,0.000635438,0.0000163027],"about_ca_topic_score_codex":0.019002724,"about_ca_topic_score_gemma":0.0091421185,"teacher_disagreement_score":0.019002724,"about_ca_system_score_codex":0.0008597469,"about_ca_system_score_gemma":0.00042022316,"threshold_uncertainty_score":0.03778428},"labels":[],"label_agreement":null},{"id":"W4403846946","doi":"10.3847/1538-4357/ad77cf","title":"Systematically Measuring Ultradiffuse Galaxies. VII. The H i Survey Overview","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy","score_opus":0.026000099269018286,"score_gpt":0.23552934362537434,"score_spread":0.20952924435635606,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403846946","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9766152,0.00505192,0.0022592875,0.00042396013,0.000034439505,0.00010606779,0.010652737,0.00017224417,0.0046841837],"genre_scores_gemma":[0.9777689,0.0023589737,0.005208666,0.00030089662,0.00005344452,0.00009790769,0.012579356,0.000031796917,0.00159996],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995912,0.000062397776,0.000041016796,0.00010035913,0.00008755942,0.00011748511],"domain_scores_gemma":[0.99807227,0.0001770765,0.00053889287,0.00023959362,0.00038236377,0.0005897339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008429335,0.0003735655,0.00025641976,0.003648905,0.00028820473,0.0006684344,0.00055863406,0.0001990808,0.0011546188],"category_scores_gemma":[0.00067398173,0.000150749,0.00021296003,0.002718215,0.00022842782,0.00054601225,0.0010562169,0.00020396769,0.00049913215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000032479424,0.000008586081,0.9795955,0.00004307887,0.00001747786,0.000028408029,0.00008141199,0.000033487493,0.0018302393,0.00009958191,0.0007429214,0.01748679],"study_design_scores_gemma":[0.000001952876,0.000035527664,0.9939592,0.000016621147,0.00001228143,0.00012737565,0.0002143915,0.000073920004,0.0008405787,0.000065080814,0.004649063,0.0000040902096],"about_ca_topic_score_codex":0.012464324,"about_ca_topic_score_gemma":0.031926513,"teacher_disagreement_score":0.012464324,"about_ca_system_score_codex":0.0004791837,"about_ca_system_score_gemma":0.00050353014,"threshold_uncertainty_score":0.024783552},"labels":[],"label_agreement":null},{"id":"W4403847087","doi":"10.3847/1538-4357/ad7135","title":"SPYGLASS. V. Spatially and Temporally Structured Star-forming Environments in the Cepheus-Hercules Complex","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Star (game theory); Astronomy; Astrophysics; Star formation; Stars","score_opus":0.014857059388032497,"score_gpt":0.2300518583328121,"score_spread":0.2151947989447796,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403847087","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9707379,0.0005539179,0.0008947602,0.00034055466,0.00004542299,0.000025408888,0.0045045572,0.00048374588,0.022413792],"genre_scores_gemma":[0.99227273,0.000120313365,0.0005022767,0.000042505293,0.000012404122,0.000013671002,0.003136813,0.00012537627,0.0037739198],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998597,0.000013903196,0.0000056909316,0.00004162854,0.000026780232,0.000052181236],"domain_scores_gemma":[0.9997869,0.00001726942,0.000067550565,0.000019502937,0.0000241591,0.00008450678],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015743192,0.00016537233,0.00019064985,0.00090608513,0.0006969998,0.0010943209,0.00024880184,0.0002262218,0.018932039],"category_scores_gemma":[0.000458633,0.00007991864,0.00009331387,0.00070585613,0.0002583141,0.00026014575,0.00081302994,0.00017728863,0.0039130854],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008340367,0.00018140729,0.6812461,0.00029278922,0.000094917596,0.0031145501,0.002274341,0.0030814938,0.020166904,0.013018911,0.047679264,0.22801544],"study_design_scores_gemma":[0.0000370479,0.00005120007,0.92271215,0.00010229087,0.00002024551,0.001263311,0.0015816134,0.0042981864,0.0009522276,0.0017979996,0.067166254,0.000017457098],"about_ca_topic_score_codex":0.021833643,"about_ca_topic_score_gemma":0.017997883,"teacher_disagreement_score":0.021833643,"about_ca_system_score_codex":0.0005631311,"about_ca_system_score_gemma":0.00031750576,"threshold_uncertainty_score":0.06333399},"labels":[],"label_agreement":null},{"id":"W4403872215","doi":"10.3847/1538-4357/ad6a14","title":"Modeling of Long-term Afterglow Counterparts to Gravitational Wave Events: The Full View of GRB 170817A","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"Ministry of Colleges and Universities; Institut Périmètre de physique théorique; Science and Technology Facilities Council; European Commission; Government of Canada; Carnegie Mellon University","keywords":"Physics; Gamma-ray burst; Afterglow; Gravitational wave; Astrophysics; Term (time); Astronomy; LIGO","score_opus":0.015621090404900565,"score_gpt":0.2596313059721242,"score_spread":0.24401021556722363,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403872215","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.930508,0.00035469496,0.06482863,0.0007724926,0.00004923553,0.000033272387,0.0006136262,0.00026184513,0.0025782436],"genre_scores_gemma":[0.9934516,0.00016915769,0.003754748,0.000068823814,0.000051392333,0.000027459006,0.0005357592,0.00006300457,0.0018780984],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99980885,0.00006580434,0.000008274949,0.000050453553,0.000020854171,0.00004584456],"domain_scores_gemma":[0.99897015,0.0004998454,0.0001921214,0.00008949484,0.00011164782,0.00013678621],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012827647,0.00060480676,0.000690949,0.00067738077,0.0005487909,0.0012432946,0.001993276,0.0013236798,0.0014494923],"category_scores_gemma":[0.0024262064,0.00051784003,0.0010512072,0.00046822403,0.0005890628,0.0012173883,0.0009388935,0.0009814196,0.00022711007],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006084269,0.000066059925,0.019436136,0.000015500249,0.00007416156,0.00013771931,0.0000539738,0.9704461,0.00093780336,0.00535199,0.00043772682,0.0029819973],"study_design_scores_gemma":[0.0000062002737,0.0000141682385,0.0024506135,0.0000022502359,0.0000123506525,0.000016935344,0.000015213628,0.99612623,0.00008634954,0.0011003069,0.00016275111,0.0000066312296],"about_ca_topic_score_codex":0.029391985,"about_ca_topic_score_gemma":0.01602293,"teacher_disagreement_score":0.029391985,"about_ca_system_score_codex":0.0008317422,"about_ca_system_score_gemma":0.00097137893,"threshold_uncertainty_score":0.05844176},"labels":[],"label_agreement":null},{"id":"W4403875515","doi":"10.3847/1538-4357/ad77c1","title":"Interpreting Mass and Radius Measurements of Neutron Stars with Dark Matter Halos","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":20,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; U.S. Department of Energy","keywords":"Physics; Halo; Dark matter; Astrophysics; Baryon; Stars; Neutron star; Astronomy; Baryonic dark matter; Dark matter halo; Galaxy","score_opus":0.012819157984433767,"score_gpt":0.2927391875054545,"score_spread":0.27992002952102074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403875515","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955978,0.00009057648,0.0031459513,0.000015700718,0.0000033659662,0.000005179587,0.0001298514,0.00008505643,0.0009265403],"genre_scores_gemma":[0.9986033,0.000020020403,0.0012111248,0.0000046195064,0.0000018640478,0.0000017135703,0.00008461192,0.000011384513,0.0000613472],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99986756,0.00004061179,0.000010005804,0.00003237703,0.00003230776,0.000017101424],"domain_scores_gemma":[0.99910647,0.00024684315,0.0003003286,0.00014941697,0.00008391186,0.00011295517],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009216772,0.00026902222,0.0002096097,0.0009372619,0.00024001753,0.00048429664,0.00034904972,0.00031936372,0.0005243154],"category_scores_gemma":[0.0023504067,0.00021803199,0.00024294732,0.0005257705,0.00035005342,0.00038849696,0.0008020866,0.0001715781,0.00012600451],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006406322,0.000042036427,0.86224544,0.000090072834,0.00017804818,0.00045995341,0.0002796455,0.061588347,0.060354773,0.003944557,0.00025957768,0.00991688],"study_design_scores_gemma":[0.000050210398,0.0001970338,0.7372946,0.000038636754,0.000098612836,0.00063211634,0.00027270702,0.21450363,0.041820094,0.0032949063,0.00174597,0.000051319996],"about_ca_topic_score_codex":0.0009315676,"about_ca_topic_score_gemma":0.0009849684,"teacher_disagreement_score":0.0009372619,"about_ca_system_score_codex":0.00039924448,"about_ca_system_score_gemma":0.000076617296,"threshold_uncertainty_score":0.0048743486},"labels":[],"label_agreement":null},{"id":"W4403899873","doi":"10.3847/1538-4357/ad7b28","title":"The Search for Disk Perturbing Planets Around the Asymmetrical Debris Disk System HD 111520 Using REBOUND","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Research Council Canada; European Space Agency","keywords":"Physics; Debris disk; Planet; Debris; Planetary system; Astronomy; Astrophysics; Protoplanetary disk; Exoplanet; Astrobiology; Planetesimal; Accretion disc; Meteorology","score_opus":0.02628238538669361,"score_gpt":0.2682084801596938,"score_spread":0.24192609477300017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403899873","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99794406,0.000018956393,0.0005809733,0.00004115651,0.0000063964253,0.000012268477,0.00018712413,0.00011563573,0.0010934321],"genre_scores_gemma":[0.99760216,0.000011481271,0.0018220508,0.000023730718,0.0000037800673,0.000010248571,0.00030903573,0.000032573185,0.00018496004],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992025,0.000016646462,0.000003046216,0.000018321836,0.000014204377,0.000027476228],"domain_scores_gemma":[0.9996258,0.00015418275,0.000052594693,0.00005618729,0.000039056406,0.000072228526],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027350435,0.0004520622,0.00035773154,0.0002976856,0.00049818034,0.00045120865,0.0010179684,0.00067006465,0.0015901021],"category_scores_gemma":[0.0007558996,0.00031538488,0.00043524578,0.00020764975,0.00037705607,0.00033059806,0.0005519013,0.000520924,0.00018530083],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006213565,0.00042582367,0.12284189,0.00013962199,0.00017893744,0.00078675203,0.00031617575,0.84715575,0.015930109,0.001810776,0.0015522864,0.008240626],"study_design_scores_gemma":[0.00016883915,0.0002976114,0.024785666,0.00001055758,0.000037224152,0.00008899692,0.00017705112,0.970301,0.0031067426,0.0003826132,0.00062682887,0.000016971873],"about_ca_topic_score_codex":0.013780258,"about_ca_topic_score_gemma":0.015098119,"teacher_disagreement_score":0.013780258,"about_ca_system_score_codex":0.0006393382,"about_ca_system_score_gemma":0.0004441246,"threshold_uncertainty_score":0.027400136},"labels":[],"label_agreement":null},{"id":"W4403900452","doi":"10.3847/1538-4357/ad7b35","title":"Star Stream Velocity Distributions in Cold Dark Matter and Warm Dark Matter Galactic Halos","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Science and Technology Council; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Tsing Hua University; University of Toronto; Durham University; Government of Ontario","keywords":"Physics; Astrophysics; Dark matter; Dark matter halo; Astronomy; Cold dark matter; Galactic halo; Scalar field dark matter; Baryonic dark matter; Cuspy halo problem; Hot dark matter; Dark fluid; Mixed dark matter; Halo; Galaxy; Cosmology; Dark energy","score_opus":0.006053855529668434,"score_gpt":0.2148541581249911,"score_spread":0.20880030259532265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403900452","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987226,0.00004455013,0.00071524875,0.000016252729,0.0000013316558,0.0000036287815,0.00017518448,0.000034232024,0.00028690428],"genre_scores_gemma":[0.999258,0.00002726067,0.00019196849,0.0000039906513,0.0000019116499,0.0000025342063,0.00036550284,0.0000083241985,0.00014043364],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999318,0.000017446344,0.000004073234,0.000019005674,0.000012271524,0.000015347441],"domain_scores_gemma":[0.9985446,0.00054293434,0.0002796857,0.000106077176,0.00026020693,0.00026651323],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059244904,0.00016491882,0.00019734226,0.0011322836,0.00019339693,0.0005982601,0.0002537985,0.00025950317,0.0011835108],"category_scores_gemma":[0.0028787341,0.00015633258,0.00023013933,0.00053509744,0.00038165468,0.00043541237,0.00035324963,0.00017316462,0.00019331451],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006304539,0.00007441648,0.7431055,0.00003814592,0.0001408916,0.00028015606,0.00034713594,0.22968777,0.010033449,0.0069740876,0.00090908306,0.0077789263],"study_design_scores_gemma":[0.00007753229,0.00015558208,0.4770661,0.0000348276,0.00003702877,0.00019080793,0.00029256448,0.5084742,0.0060454067,0.0063857883,0.0011618482,0.00007831541],"about_ca_topic_score_codex":0.0055322675,"about_ca_topic_score_gemma":0.0035909894,"teacher_disagreement_score":0.0055322675,"about_ca_system_score_codex":0.0007197672,"about_ca_system_score_gemma":0.00021423983,"threshold_uncertainty_score":0.011000156},"labels":[],"label_agreement":null},{"id":"W4403984333","doi":"10.3847/1538-4357/ad7b12","title":"On the Role of Noncircular Motions in MaNGA Galaxies. I. Global Properties","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; York University; Ministry of Science and Technology, Taiwan; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; National Science and Technology Council; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik; Academia Sinica; European Commission","keywords":"Physics; Galaxy; Astrophysics; Astronomy; Galaxy formation and evolution","score_opus":0.007888846675869188,"score_gpt":0.20134795451895937,"score_spread":0.19345910784309017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4403984333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986546,0.00019158708,0.00018240564,0.000018217279,0.0000014657362,0.0000032684807,0.00023223774,0.0000094071975,0.0007068512],"genre_scores_gemma":[0.9996424,0.000022543842,0.00007554241,0.0000032940359,0.0000030224082,0.0000012626301,0.00016487035,0.0000032941427,0.0000838974],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99976057,0.000044015742,0.000013377652,0.00009912472,0.00003074236,0.000052205425],"domain_scores_gemma":[0.9972566,0.00075492787,0.0010299396,0.00043372044,0.00023348312,0.00029137253],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00051419024,0.00022895834,0.00022658793,0.0013104561,0.0003848743,0.00046518975,0.00028298298,0.00016703937,0.0011097023],"category_scores_gemma":[0.0015159234,0.00014452256,0.00020877419,0.00093349966,0.0006197908,0.0004716817,0.0004855509,0.0001825176,0.000218579],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000024342016,0.00000540221,0.99468577,0.000007261465,0.000016290096,0.000022924485,0.00010739772,0.0001534505,0.0027993948,0.000059189053,0.000033693366,0.0020849237],"study_design_scores_gemma":[5.997042e-7,0.0000088891975,0.99936956,0.0000011900162,0.000004934206,0.000019046453,0.000040257015,0.00023578461,0.00020653,0.00002154891,0.00009061769,0.0000010236581],"about_ca_topic_score_codex":0.007828008,"about_ca_topic_score_gemma":0.011988334,"teacher_disagreement_score":0.007828008,"about_ca_system_score_codex":0.000361608,"about_ca_system_score_gemma":0.00014190708,"threshold_uncertainty_score":0.015564859},"labels":[],"label_agreement":null},{"id":"W4404024622","doi":"10.3847/1538-4357/ad7d90","title":"Cross-correlating Dark Sirens and Galaxies: Constraints on H <sub>0</sub> from GWTC-3 of LIGO–Virgo–KAGRA","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Perimeter Institute","funders":"Science and Technology Facilities Council; Institut Périmètre de physique théorique; Centre National de la Recherche Scientifique; National Science Foundation; Government of Canada; Ministry of Colleges and Universities","keywords":"Physics; Galaxy; Astrophysics; LIGO; Gravitational wave","score_opus":0.010684565659313706,"score_gpt":0.30605761123081693,"score_spread":0.29537304557150323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404024622","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98222876,0.00012214965,0.012017015,0.00005230345,0.0000050965286,0.000009900818,0.0019334912,0.00029790003,0.0033332817],"genre_scores_gemma":[0.9940252,0.000035221266,0.0027493732,0.000026292535,0.000012660046,0.000009290721,0.002852787,0.000059539172,0.00022960737],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997008,0.0000619764,0.000015936634,0.000077728044,0.0000780717,0.00006553515],"domain_scores_gemma":[0.9965718,0.0011091963,0.0008526946,0.000704056,0.00029711585,0.00046507662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014474853,0.00034568977,0.00024480678,0.0020234047,0.00020970605,0.0006121137,0.00029124925,0.0002757225,0.0019524021],"category_scores_gemma":[0.0028216855,0.00021682151,0.0004396662,0.0012969058,0.00032557207,0.00028190127,0.0010002075,0.00025255128,0.0006829212],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002556745,0.000034005283,0.9561681,0.000031423482,0.00016406733,0.00012539305,0.00012880322,0.0052634124,0.013877556,0.001663383,0.0011462783,0.021142058],"study_design_scores_gemma":[0.000014925168,0.000029038292,0.97508293,0.000008818816,0.000049501858,0.00013233708,0.00005503488,0.016731506,0.0057518804,0.00089418486,0.0012350109,0.000014808031],"about_ca_topic_score_codex":0.00521767,"about_ca_topic_score_gemma":0.008283565,"teacher_disagreement_score":0.00521767,"about_ca_system_score_codex":0.00023888926,"about_ca_system_score_gemma":0.00024316329,"threshold_uncertainty_score":0.010374606},"labels":[],"label_agreement":null},{"id":"W4404044612","doi":"10.3847/1538-4357/ad79ec","title":"TEMPLATES: Direct Abundance Constraints for Two Lensed Lyman-break Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Dalhousie University; Herzberg Institute of Astrophysics","funders":"Goddard Space Flight Center; Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Abundance (ecology); Astronomy; Luminous infrared galaxy; Galaxy formation and evolution; Disc; Radio galaxy","score_opus":0.017828799519170904,"score_gpt":0.30431081721138736,"score_spread":0.2864820176922165,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404044612","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9867214,0.000067377216,0.006044348,0.000030225745,0.000004743069,0.000026354817,0.0047934214,0.00040388972,0.0019083276],"genre_scores_gemma":[0.9811933,0.000022542983,0.0060285535,0.000015651163,0.000008928869,0.000017927725,0.012377943,0.00005126521,0.00028403435],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99950683,0.000049902916,0.000037394955,0.00017779753,0.00014870564,0.000079338955],"domain_scores_gemma":[0.99812967,0.0004561521,0.00042279004,0.00041817292,0.00025639992,0.00031684447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007522481,0.00039594172,0.00034511287,0.0011894153,0.00033340015,0.0010112571,0.0007962063,0.00046526606,0.0020701508],"category_scores_gemma":[0.004134498,0.000294228,0.00052849075,0.00077679654,0.00020493889,0.0004207354,0.0006570422,0.00027568938,0.00064174534],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004890848,0.00016969604,0.91651523,0.000043458655,0.00030476094,0.00023712088,0.000093840885,0.023720235,0.034967944,0.0023334776,0.0020885842,0.019036619],"study_design_scores_gemma":[0.00013171688,0.00013501289,0.7985941,0.000012311181,0.00011049168,0.00027502124,0.00010271943,0.1750289,0.02081695,0.0018855906,0.002872606,0.000034677116],"about_ca_topic_score_codex":0.030008957,"about_ca_topic_score_gemma":0.04423981,"teacher_disagreement_score":0.030008957,"about_ca_system_score_codex":0.00088557875,"about_ca_system_score_gemma":0.00047333536,"threshold_uncertainty_score":0.0596686},"labels":[],"label_agreement":null},{"id":"W4404063438","doi":"10.3847/1538-4357/ad7f50","title":"Binary Disruption and Ejected Stars from Hierarchical Star Cluster Assembly","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Supercomputing Center, Korea Institute of Science and Technology Information; Alliance de recherche numérique du Canada; Natural Sciences and Engineering Research Council of Canada; Universiteit Leiden","keywords":"Physics; Stars; Star cluster; Astrophysics; Binary star; Cluster (spacecraft); Astronomy; Star (game theory); Binary number; Blue straggler","score_opus":0.009758168066625016,"score_gpt":0.2379199161959481,"score_spread":0.22816174812932308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404063438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99839646,0.000025050404,0.0004382382,0.000030991767,0.0000047217936,0.000008106163,0.00005962333,0.000026115582,0.001010697],"genre_scores_gemma":[0.99935573,0.000016919685,0.00031849262,0.000016213184,0.0000014727419,0.0000053192803,0.00007877136,0.00001018671,0.00019687515],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997917,0.0000445477,0.000010272102,0.000029504046,0.000049092232,0.00007497868],"domain_scores_gemma":[0.9991653,0.00031057556,0.0001719211,0.00006684474,0.00008627087,0.00019924015],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003524527,0.00039741516,0.0003420773,0.00043618964,0.0007926075,0.0009586534,0.0007688254,0.000573334,0.001495149],"category_scores_gemma":[0.0024459288,0.00031437204,0.0004223484,0.00044675719,0.00081335386,0.00044032617,0.001028041,0.0004868871,0.00014689362],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020270878,0.00013445235,0.03957043,0.00002750514,0.000077327386,0.00024088497,0.00017217277,0.95207167,0.0041808668,0.0016550384,0.00023348109,0.0014335362],"study_design_scores_gemma":[0.00016295222,0.00025363182,0.021510763,0.000012636705,0.000049427486,0.000085751126,0.00019570347,0.972715,0.0033278032,0.0011254448,0.0005342009,0.000026531823],"about_ca_topic_score_codex":0.026451632,"about_ca_topic_score_gemma":0.019470356,"teacher_disagreement_score":0.026451632,"about_ca_system_score_codex":0.0017493523,"about_ca_system_score_gemma":0.0008849123,"threshold_uncertainty_score":0.052595377},"labels":[],"label_agreement":null},{"id":"W4404063446","doi":"10.3847/1538-4357/ad77cc","title":"Forecasts and Statistical Insights for Line Intensity Mapping Cross-correlations: A Case Study with 21 cm × [C ii]","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Fonds de recherche du Québec – Nature et technologies","keywords":"Physics; Intensity mapping; Intensity (physics); Line (geometry); Astrophysics; Statistical analysis; Statistical physics; Computational physics; Statistics; Optics; Geometry; Galaxy","score_opus":0.021529074584111414,"score_gpt":0.2784211124538598,"score_spread":0.2568920378697484,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404063446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6449813,0.00040811813,0.3468533,0.0022814998,0.00005839163,0.00009610577,0.00096135604,0.0006194445,0.0037404997],"genre_scores_gemma":[0.9523369,0.00013494858,0.045605917,0.00008776835,0.000048530324,0.00003580723,0.0005502902,0.00011928427,0.0010806498],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99891424,0.00044422838,0.000051226452,0.0002809636,0.00017729957,0.00013205624],"domain_scores_gemma":[0.97419655,0.019781614,0.0018993398,0.0012387407,0.0022363306,0.00064735685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00793111,0.0006589128,0.0006303807,0.0011118376,0.00070391136,0.0017280253,0.0014833969,0.0014982981,0.0021285557],"category_scores_gemma":[0.0317435,0.00051795284,0.0006280745,0.0011334799,0.00085479225,0.0020728162,0.0013391082,0.001982333,0.00023991002],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000703156,0.00006867423,0.042701375,0.000028727449,0.000036127603,0.00049196155,0.00021278778,0.91709286,0.0006988367,0.024864428,0.0016574009,0.012076526],"study_design_scores_gemma":[0.0000043010878,0.000009935413,0.0021284411,0.000005203821,0.000004077804,0.000026459738,0.00003656047,0.99063736,0.00021079405,0.006675727,0.0002516718,0.00000938374],"about_ca_topic_score_codex":0.03555975,"about_ca_topic_score_gemma":0.02435426,"teacher_disagreement_score":0.03555975,"about_ca_system_score_codex":0.001443947,"about_ca_system_score_gemma":0.0011683924,"threshold_uncertainty_score":0.07070553},"labels":[],"label_agreement":null},{"id":"W4404112966","doi":"10.3847/1538-4357/ad7c42","title":"The SDSS-V Black Hole Mapper Reverberation Mapping Project: A Kinematically Variable Broad-line Region and Consequences for the Masses of Luminous Quasars","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"National Science Foundation","keywords":"Physics; Reverberation mapping; Quasar; Astrophysics; Astronomy; Black hole (networking); Line (geometry); Variable star; Stars; Galaxy","score_opus":0.018486821527585393,"score_gpt":0.24819574450971463,"score_spread":0.22970892298212925,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404112966","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99827087,0.000022321701,0.00046438977,0.000019447232,0.0000016719752,0.0000035198996,0.0008249533,0.00004060173,0.00035210763],"genre_scores_gemma":[0.99672616,0.000012099594,0.0008252438,0.0000073351994,0.0000033140718,0.0000046477307,0.0021576607,0.000021738288,0.00024168975],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996573,0.000070965034,0.000013909014,0.00010270609,0.00008967903,0.00006536208],"domain_scores_gemma":[0.9990682,0.00015480745,0.00036941186,0.00015800686,0.000109031236,0.00014056612],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00087348884,0.00028326234,0.00018150843,0.0009737812,0.00027620269,0.0007249443,0.00033242992,0.00021712254,0.000866371],"category_scores_gemma":[0.0015562397,0.0001329907,0.00023590874,0.00068831607,0.00019241052,0.00036003202,0.0005876889,0.00021937635,0.00031130007],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003004248,0.00008882912,0.9735218,0.000012619716,0.000058442638,0.00020172453,0.00030719885,0.001605111,0.011864758,0.00021868545,0.0005503268,0.011270111],"study_design_scores_gemma":[0.0000038327285,0.000023832623,0.995576,0.0000024590054,0.0000069412667,0.00007430239,0.00011076917,0.0024848485,0.0012299115,0.000054103537,0.00042968758,0.0000034141406],"about_ca_topic_score_codex":0.005499522,"about_ca_topic_score_gemma":0.005453688,"teacher_disagreement_score":0.005499522,"about_ca_system_score_codex":0.00017096975,"about_ca_system_score_gemma":0.00013720253,"threshold_uncertainty_score":0.0109350085},"labels":[],"label_agreement":null},{"id":"W4404115161","doi":"10.3847/1538-4357/ad7dea","title":"Estimating Dust Attenuation from Galactic Spectra. III. Radial Variations of Dust Attenuation Scaling Relations in MaNGA Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Smithsonian Astrophysical Observatory; University of Colorado Boulder; Office of Science; Max-Planck-Institut für Astronomie; Ministério da Ciência, Tecnologia e Inovação; U.S. Department of Energy; Smithsonian Institution; National Natural Science Foundation of China; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; National Key Research and Development Program of China; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Astrophysics; Attenuation; Galaxy; Extinction (optical mineralogy); Scaling; Spectral line; Astronomy; Optics","score_opus":0.01090966016251945,"score_gpt":0.23299049922208565,"score_spread":0.2220808390595662,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404115161","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997519,0.00012361656,0.0015858865,0.000011512658,0.0000010438156,0.000002985756,0.0002147346,0.00007547489,0.0004658384],"genre_scores_gemma":[0.9990814,0.000025719528,0.00059959054,0.0000021417216,0.0000020004932,0.0000016008127,0.00020972129,0.000007451421,0.0000704176],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986637,0.000022852497,0.000008326257,0.00004451646,0.00003078681,0.000027207227],"domain_scores_gemma":[0.99874026,0.0004044766,0.00040855308,0.00014820199,0.00020389029,0.00009454293],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004275882,0.0003367733,0.00017352594,0.0018189498,0.00017378591,0.00037942038,0.00017889556,0.00019302516,0.00053879846],"category_scores_gemma":[0.0019694862,0.00015744228,0.00024949785,0.00073712366,0.00020810521,0.00032210222,0.00026563066,0.00017842674,0.00033130293],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006089776,0.000016968417,0.9667545,0.000018458819,0.000048458343,0.000052047395,0.000093209426,0.0030728048,0.017083183,0.000078564415,0.000066181914,0.012654702],"study_design_scores_gemma":[0.000001201662,0.000013576464,0.9900624,0.0000030159547,0.000009435008,0.00003999088,0.0000445195,0.007872869,0.0017719253,0.000060847695,0.00011642222,0.0000038601734],"about_ca_topic_score_codex":0.0061960635,"about_ca_topic_score_gemma":0.005777,"teacher_disagreement_score":0.0061960635,"about_ca_system_score_codex":0.00022100363,"about_ca_system_score_gemma":0.000074978096,"threshold_uncertainty_score":0.012319982},"labels":[],"label_agreement":null},{"id":"W4404123520","doi":"10.3847/1538-4357/ad7a7b","title":"A Systematic Analysis of Star Cluster Disruption by Tidal Shocks. II. Predicting Star Cluster Dissolution Rates from a Time-series Analysis of Their Tidal Histories","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University; York University; University of Toronto","funders":"Medical Research Council; European Commission; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Theoretical Astrophysics; Compute Canada; Canadian Network for Research and Innovation in Machining Technology, Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Star cluster; Cluster (spacecraft); Spectral density; Population; Star formation; Galaxy; Statistics; Demography","score_opus":0.00620311543903759,"score_gpt":0.22034666107447987,"score_spread":0.21414354563544227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404123520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979657,0.000018687126,0.0017178563,0.00001885925,0.0000021677063,0.000008489658,0.0000977059,0.00002838224,0.0001421214],"genre_scores_gemma":[0.9980926,0.000016005779,0.0015353896,0.0000060632783,0.0000019930849,0.00001079243,0.00025915474,0.000007698326,0.000070344686],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999869,0.000047682763,0.000009860635,0.000033460474,0.000022723963,0.000017239194],"domain_scores_gemma":[0.9988067,0.0006285655,0.00018464975,0.0001687713,0.00012923198,0.00008204699],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007767728,0.0002752841,0.00023664904,0.0005877681,0.0003638876,0.00027002208,0.0005197726,0.00038720213,0.00032997117],"category_scores_gemma":[0.002535297,0.00023955732,0.0006881426,0.00037690153,0.0004039126,0.00034256637,0.00033209223,0.00034133735,0.00004902276],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015033032,0.00018418084,0.1611398,0.000042762495,0.00023336991,0.00016450486,0.00011163294,0.8178684,0.013051387,0.0013772561,0.00027259937,0.0054038437],"study_design_scores_gemma":[0.000014845543,0.000080273385,0.029354228,0.0000027667745,0.000019208539,0.00002835956,0.000026279507,0.9678583,0.0021347462,0.0003731769,0.00009986136,0.0000079458005],"about_ca_topic_score_codex":0.008326631,"about_ca_topic_score_gemma":0.008082988,"teacher_disagreement_score":0.008326631,"about_ca_system_score_codex":0.00058701454,"about_ca_system_score_gemma":0.00038218952,"threshold_uncertainty_score":0.016556323},"labels":[],"label_agreement":null},{"id":"W4404135094","doi":"10.3847/1538-4357/ad81f7","title":"Hydrodynamical Simulations of Proton Ingestion Flashes in Type I X-Ray Bursts","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; McGill University Health Centre","funders":"Natural Sciences and Engineering Research Council of Canada; Stony Brook University; National Energy Research Scientific Computing Center","keywords":"Physics; Astrophysics; Proton; Astronomy; Nuclear physics","score_opus":0.011100465751630727,"score_gpt":0.2557091816590128,"score_spread":0.24460871590738206,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404135094","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.991836,0.0000853586,0.0017094327,0.00028966277,0.000042832147,0.000048123642,0.00037767188,0.00011383813,0.005497046],"genre_scores_gemma":[0.9969361,0.000054868797,0.0014999758,0.00008809565,0.000014263944,0.00004890251,0.0003070269,0.00004525685,0.0010055492],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999778,0.000056890425,0.000012498002,0.000023358763,0.000043402015,0.00008585129],"domain_scores_gemma":[0.9984389,0.00083540904,0.00016667288,0.00007281128,0.00016712572,0.00031911087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052339764,0.00065582915,0.00081121986,0.0006958486,0.0010547548,0.0011716244,0.001128116,0.0017079714,0.0028155271],"category_scores_gemma":[0.0026268149,0.000519468,0.00085643015,0.0005428329,0.0015303451,0.000653672,0.0010442293,0.0012264211,0.00019842054],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002471051,0.00024807177,0.010272351,0.000031838455,0.00007644039,0.00026907015,0.0001417677,0.9836817,0.0016105413,0.0018060401,0.0004422923,0.0011727568],"study_design_scores_gemma":[0.000071602364,0.00005600503,0.0020504962,0.0000075635276,0.000008756468,0.000012951653,0.000090705355,0.99679,0.0004109453,0.00030509415,0.00018638084,0.000009436286],"about_ca_topic_score_codex":0.024051318,"about_ca_topic_score_gemma":0.01133472,"teacher_disagreement_score":0.024051318,"about_ca_system_score_codex":0.0016220261,"about_ca_system_score_gemma":0.0011438723,"threshold_uncertainty_score":0.047822654},"labels":[],"label_agreement":null},{"id":"W4404146413","doi":"10.3847/1538-4357/ad6c4f","title":"3D Hydrodynamic Simulations of Massive Main-sequence Stars. III. The Effect of Radiation Pressure and Diffusion Leading to a 1D Equilibrium Model","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Science Foundation","keywords":"Physics; Radiation pressure; Diffusion; Stars; Sequence (biology); Main sequence; Statistical physics; Astrophysics; Radiation transport; Radiation; Classical mechanics; Mechanics; Thermodynamics; Monte Carlo method; Nuclear physics","score_opus":0.007997772863107112,"score_gpt":0.2456887336454379,"score_spread":0.2376909607823308,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404146413","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9879358,0.000100134996,0.005616481,0.00025107857,0.000037349906,0.000044897148,0.0004460296,0.00018989439,0.0053784177],"genre_scores_gemma":[0.99389666,0.00006789074,0.0043560416,0.000080298196,0.000016395983,0.000063638065,0.0003994287,0.00005827657,0.001061359],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998449,0.000040929426,0.0000075835105,0.000016759193,0.00004055727,0.000049172486],"domain_scores_gemma":[0.99936813,0.00025534997,0.00007597035,0.000048023147,0.00010191914,0.00015054143],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042086898,0.0005300587,0.0006725797,0.00039194312,0.0007809868,0.0007610643,0.0009419988,0.0012381816,0.0015833947],"category_scores_gemma":[0.0015823208,0.00036328466,0.00093272707,0.00040826356,0.00088060286,0.00042849244,0.0007625598,0.00082010985,0.00024280489],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000859494,0.000058138034,0.0030164004,0.000018611438,0.000020999787,0.000088220295,0.00006235986,0.99289274,0.0015653544,0.0011201366,0.00021264283,0.0008584816],"study_design_scores_gemma":[0.00003448638,0.000032270433,0.0009573157,0.000003896013,0.0000039149113,0.000007897463,0.000016134332,0.9981651,0.00034522265,0.00030851172,0.00012002872,0.0000052271025],"about_ca_topic_score_codex":0.02079457,"about_ca_topic_score_gemma":0.009291287,"teacher_disagreement_score":0.02079457,"about_ca_system_score_codex":0.0013651535,"about_ca_system_score_gemma":0.0010560453,"threshold_uncertainty_score":0.041347086},"labels":[],"label_agreement":null},{"id":"W4404147652","doi":"10.3847/1538-4357/ad77bc","title":"Probing Populations of Dark Stellar Remnants in the Globular Clusters 47 Tuc and Terzan 5 Using Pulsar Timing","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Globular cluster; Physics; Astrophysics; Astronomy; Pulsar; Galaxy","score_opus":0.03354118698088902,"score_gpt":0.2769174019314974,"score_spread":0.24337621495060835,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404147652","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975293,0.000022654429,0.0014891914,0.00001082836,0.0000013944596,0.0000037791858,0.00021013105,0.00005081628,0.00068181613],"genre_scores_gemma":[0.99707556,0.0000125703555,0.0022882945,0.0000038965363,0.0000021042501,0.000004860365,0.00038894903,0.000017908314,0.00020585107],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999182,0.000014063694,0.0000025823083,0.000028892266,0.00001638688,0.000019845153],"domain_scores_gemma":[0.9996345,0.00008313128,0.00007887212,0.00006222885,0.000060770162,0.000080427344],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003696497,0.0002111287,0.00027898554,0.0011539096,0.00036680524,0.0006046921,0.00043317128,0.00028890543,0.0009023843],"category_scores_gemma":[0.00094782904,0.000191124,0.00028538104,0.0006659492,0.00021375544,0.0002546415,0.000506429,0.0001576138,0.00026719453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026501296,0.000041370164,0.9169572,0.00001873612,0.00014286659,0.000120160206,0.00037996392,0.032551777,0.033466216,0.0013956833,0.00041102275,0.014249953],"study_design_scores_gemma":[0.000023193776,0.00006894546,0.74884444,0.000009763329,0.00006336199,0.000096462296,0.00030783648,0.24121356,0.007185594,0.0007763017,0.001377109,0.0000335517],"about_ca_topic_score_codex":0.026223363,"about_ca_topic_score_gemma":0.030304767,"teacher_disagreement_score":0.026223363,"about_ca_system_score_codex":0.0011693531,"about_ca_system_score_gemma":0.00033549065,"threshold_uncertainty_score":0.052141428},"labels":[],"label_agreement":null},{"id":"W4404147825","doi":"10.3847/1538-4357/ad7a6f","title":"Dual Active Galactic Nuclei: Precursors of Binary Supermassive Black Hole Formation and Mergers","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Natural Sciences and Engineering Research Council of Canada; Infosys Foundation; Alliance de recherche numérique du Canada; Department of Atomic Energy, Government of India; Ames Research Center; University of Illinois at Urbana-Champaign; Leverhulme Trust; Tata Institute of Fundamental Research; Western Canada Research Grid; Indian Institute of Science; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Supermassive black hole; Astrophysics; Active galactic nucleus; Binary black hole; Binary number; Intermediate-mass black hole; Astronomy; Galactic nuclei; Gamma-ray burst progenitors; Stellar black hole; Galaxy; Gravitational wave","score_opus":0.011541211783244167,"score_gpt":0.23589388155742308,"score_spread":0.22435266977417892,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404147825","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983877,0.000092954135,0.00073795224,0.00003510507,0.0000031045759,0.000003969431,0.00007965109,0.000020934724,0.0006386073],"genre_scores_gemma":[0.99955493,0.000015777321,0.00027899267,0.000006197572,0.0000024846395,0.0000013221317,0.000060784685,0.000003510114,0.00007594239],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977607,0.000043432734,0.000011230703,0.0000815011,0.000047488644,0.000040417908],"domain_scores_gemma":[0.99881905,0.0003007024,0.0004615187,0.00008175042,0.00005302896,0.0002840002],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039608288,0.00025184432,0.0003213051,0.00077166554,0.0003635225,0.0010572915,0.00042576768,0.00038563745,0.0021745367],"category_scores_gemma":[0.0020019438,0.00023184043,0.00039485877,0.00038601243,0.00049755484,0.00047934862,0.00084609113,0.00039092143,0.0001421674],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024591284,0.00005791322,0.96752685,0.000034091885,0.00010350095,0.0010140351,0.0001649157,0.00868078,0.014205096,0.0031060784,0.00020275093,0.004658029],"study_design_scores_gemma":[0.000037943286,0.00008354144,0.9079079,0.000013944637,0.00006991922,0.0014405025,0.0002747871,0.08153226,0.004940648,0.002867046,0.00080733316,0.000024195211],"about_ca_topic_score_codex":0.0030927483,"about_ca_topic_score_gemma":0.0027510358,"teacher_disagreement_score":0.0030927483,"about_ca_system_score_codex":0.00045693095,"about_ca_system_score_gemma":0.00018100272,"threshold_uncertainty_score":0.0072745085},"labels":[],"label_agreement":null},{"id":"W4404149531","doi":"10.3847/1538-4357/ad77c7","title":"Magnetic Field Alignment Relative to Multiple Tracers in the High-mass Star-forming Region RCW 36","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"RES’EAU-WaterNET; Queen's University; Universities Space Research Association; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Star (game theory); Magnetic field; Astronomy; Field (mathematics)","score_opus":0.011693571761915997,"score_gpt":0.23959684679291973,"score_spread":0.22790327503100374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404149531","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864393,0.000021644319,0.00007335634,0.000007917953,0.0000015558354,0.000003099981,0.00072833564,0.000028392917,0.0004917895],"genre_scores_gemma":[0.99875855,0.00001478813,0.000181289,0.000004050545,0.0000030292429,0.0000024158808,0.00095526536,0.000008021205,0.00007257444],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987996,0.000007973435,0.0000058590363,0.00003716898,0.000028269764,0.000040811356],"domain_scores_gemma":[0.99967337,0.0000309149,0.0001095903,0.000038767765,0.000060844606,0.000086406486],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017368834,0.00020392238,0.0003206536,0.0011372035,0.00027051836,0.00049461314,0.00024793964,0.00022358962,0.0006563456],"category_scores_gemma":[0.00043643088,0.00014639247,0.00020230605,0.00091560284,0.00022491804,0.00014674605,0.00031811753,0.00020084268,0.0002893699],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048082287,0.00007248465,0.87049395,0.000042549764,0.00009879143,0.00043147325,0.00046644523,0.0039377254,0.11208083,0.00011144429,0.00053539756,0.011248135],"study_design_scores_gemma":[0.000007912806,0.000024673325,0.9957767,0.0000032474086,0.000010574113,0.000070327595,0.0000803072,0.0015591078,0.0021449043,0.000021953514,0.0002945353,0.00000569133],"about_ca_topic_score_codex":0.02284334,"about_ca_topic_score_gemma":0.023402927,"teacher_disagreement_score":0.02284334,"about_ca_system_score_codex":0.0005153355,"about_ca_system_score_gemma":0.00024342285,"threshold_uncertainty_score":0.045420766},"labels":[],"label_agreement":null},{"id":"W4404194147","doi":"10.3847/1538-4357/ad7ff0","title":"Astrometric Jitter as a Detection Diagnostic for Recoiling and Slingshot Supermassive Black Hole Candidates","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Los Alamos National Laboratory; Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Queen's University Belfast; W. M. Keck Foundation; Space Telescope Science Institute; Queen's University; NASA Exoplanet Science Institute; Johns Hopkins University; Harvard University; John Templeton Foundation; National Central University; Gordon and Betty Moore Foundation; Eötvös Loránd Tudományegyetem; California Institute of Technology; National Aeronautics and Space Administration; Durham University; Smithsonian Institution; National Science Foundation","keywords":"Physics; Supermassive black hole; Jitter; Astrophysics; Astronomy; Galaxy","score_opus":0.011241821302935474,"score_gpt":0.2443473929159287,"score_spread":0.23310557161299322,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404194147","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980286,0.000068408284,0.0005194615,0.000016960907,0.0000041232306,0.0000072397734,0.00024617155,0.00007654646,0.0010325175],"genre_scores_gemma":[0.9987117,0.000022561399,0.00082571595,0.0000062476283,0.000004477071,0.0000025345364,0.00027395703,0.0000070224014,0.00014572134],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997607,0.00003719628,0.000020262843,0.000061872335,0.00006333264,0.000056702305],"domain_scores_gemma":[0.9985593,0.0002805864,0.00061751774,0.00011547333,0.0001362013,0.0002908622],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00056361087,0.00018419087,0.00018205788,0.0030778942,0.00018586034,0.0005113885,0.0003054989,0.00018386853,0.0014349752],"category_scores_gemma":[0.0015183013,0.00011104998,0.00014266714,0.0009168298,0.00020862433,0.00023316141,0.00048003017,0.00014610896,0.00028824125],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000099097146,0.000009243121,0.98786724,0.000006334295,0.000011347936,0.000111477326,0.000082909064,0.0002660047,0.004479774,0.00007889916,0.00019840316,0.0067893295],"study_design_scores_gemma":[0.0000028870681,0.000034349763,0.997166,0.0000035655057,0.000009221137,0.00021387904,0.00007568607,0.0012226418,0.001006853,0.000033034667,0.00022810033,0.0000038002636],"about_ca_topic_score_codex":0.0036595264,"about_ca_topic_score_gemma":0.008026055,"teacher_disagreement_score":0.0036595264,"about_ca_system_score_codex":0.00022340019,"about_ca_system_score_gemma":0.0000820725,"threshold_uncertainty_score":0.007276416},"labels":[],"label_agreement":null},{"id":"W4404220035","doi":"10.3847/1538-4357/ad8233","title":"Shadows Wreak Havoc in Transition Disks","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astronomy; Astrophysics; Astrobiology","score_opus":0.010369714371952886,"score_gpt":0.24900061677269025,"score_spread":0.23863090240073737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404220035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99599886,0.00014696985,0.001238279,0.00013501036,0.000025257712,0.000009297332,0.0000914161,0.00009256428,0.0022623667],"genre_scores_gemma":[0.9993767,0.000026460848,0.00032185257,0.000025811425,0.000005397464,0.000002866555,0.000044523433,0.000022770295,0.00017371323],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99988115,0.000020077303,0.0000045043394,0.000021920128,0.000017481918,0.000054794178],"domain_scores_gemma":[0.9996253,0.00013006225,0.00005024413,0.00004642145,0.000027631148,0.00012026314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022030156,0.00036194027,0.00051782175,0.0003925212,0.00089235196,0.0016036257,0.0005296097,0.0007178786,0.0024006218],"category_scores_gemma":[0.0013300406,0.00030174854,0.0005004525,0.00022206696,0.0010830913,0.0009277707,0.0011661457,0.0006272984,0.00017108717],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012731345,0.00041616737,0.04928825,0.0001805205,0.0002020789,0.0019003282,0.0010392626,0.89543635,0.032438207,0.008010228,0.0021384005,0.0076770238],"study_design_scores_gemma":[0.00030426044,0.00028761697,0.024993198,0.00003472575,0.00006466277,0.0002610703,0.00067835674,0.96263504,0.0037131237,0.0049466435,0.0020218624,0.00005954219],"about_ca_topic_score_codex":0.009043385,"about_ca_topic_score_gemma":0.0038469797,"teacher_disagreement_score":0.009043385,"about_ca_system_score_codex":0.0006717793,"about_ca_system_score_gemma":0.0004297876,"threshold_uncertainty_score":0.01798153},"labels":[],"label_agreement":null},{"id":"W4404242693","doi":"10.3847/1538-4357/ad812f","title":"Search for Joint Multimessenger Signals from Potential Galactic Cosmic-Ray Accelerators with HAWC and IceCube","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"Institute for Cosmic Ray Research, University of Tokyo; Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Los Alamos National Laboratory; Office of Polar Programs; College of Engineering, Michigan State University; Goddard Space Flight Center; Office of National Higher Education Science Research and Innovation Policy Council; Helmholtz Alliance for Astroparticle Physics; Alliance de recherche numérique du Canada; Chiba University; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Office of Experimental Program to Stimulate Competitive Research; Benemérita Universidad Autónoma de Puebla; Knut och Alice Wallenbergs Stiftelse; Coordinación de la Investigación Científica; Villum Fonden; National Research Foundation of Korea; Consejo Nacional de Ciencia y Tecnología; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Laboratory Directed Research and Development; National Science Foundation; Belgian Federal Science Policy Office; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Deutsche Forschungsgemeinschaft; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Deutsches Elektronen-Synchrotron; Generalitat Valenciana; Marquette University; Fonds Wetenschappelijk Onderzoek; Nvidia; National Aeronautics and Space Administration; National Research Foundation; Michigan State University","keywords":"Physics; Neutrino; Cosmic ray; Astrophysics; Gamma ray; Flux (metallurgy); COSMIC cancer database; Astronomy; Neutrino astronomy; Neutrino detector; Neutrino oscillation; Nuclear physics","score_opus":0.014220827535182504,"score_gpt":0.24074663731160045,"score_spread":0.22652580977641795,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404242693","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9825095,0.00016216042,0.010902854,0.0000699581,0.00001101811,0.000031554424,0.0024437297,0.00047165394,0.0033976105],"genre_scores_gemma":[0.9824949,0.00003855464,0.010152807,0.000036319903,0.00001607894,0.000032205804,0.006616539,0.00010133441,0.0005113628],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9987909,0.0003922791,0.000049045007,0.00031518764,0.00031139862,0.0001412035],"domain_scores_gemma":[0.9939067,0.0031731313,0.0012783554,0.00065243826,0.00058992155,0.0003994975],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0036238455,0.0003493918,0.0005894248,0.0021629662,0.00051864004,0.001449406,0.0005453936,0.00039871602,0.0021915117],"category_scores_gemma":[0.0055114194,0.0003024003,0.0006239182,0.0019426579,0.00035059918,0.00045072273,0.001191167,0.00048581345,0.00029812014],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004885981,0.000053812233,0.96322876,0.000038171762,0.0003601535,0.00025668464,0.00013357976,0.012737338,0.005647286,0.0015216433,0.0011960629,0.014338],"study_design_scores_gemma":[0.00007410686,0.00020294295,0.8815327,0.000041115192,0.00018511376,0.0005581167,0.00017807056,0.09736299,0.0122198975,0.0017394881,0.0058625056,0.00004299415],"about_ca_topic_score_codex":0.0039185965,"about_ca_topic_score_gemma":0.0059759156,"teacher_disagreement_score":0.0039185965,"about_ca_system_score_codex":0.00070019613,"about_ca_system_score_gemma":0.00079501595,"threshold_uncertainty_score":0.01916492},"labels":[],"label_agreement":null},{"id":"W4404297502","doi":"10.3847/1538-4357/ad7a73","title":"High-redshift, Small-scale Tests of Ultralight Axion Dark Matter Using Hubble and Webb Galaxy UV Luminosities","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Connaught Fund; University of Toronto; Leverhulme Trust; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Canadian Institute for Advanced Research","keywords":"Physics; Astrophysics; Dark matter; Astronomy; Galaxy; Redshift; Axion","score_opus":0.009138695177305175,"score_gpt":0.22302668009679782,"score_spread":0.21388798491949265,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404297502","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965784,0.000058387133,0.0017152302,0.000025895348,0.0000030281383,0.0000034562677,0.00039654796,0.00007942353,0.0011397057],"genre_scores_gemma":[0.99915314,0.000007226321,0.00036976085,0.000008121773,0.000003209717,0.0000037072616,0.00027982416,0.000013711998,0.00016130702],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993869,0.00024200515,0.00002428315,0.00015148874,0.00011328845,0.000082037826],"domain_scores_gemma":[0.99432725,0.0030398085,0.0010582996,0.0006386931,0.00025747824,0.00067851495],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017052151,0.00037719824,0.0002502204,0.0014954482,0.00028193434,0.00094309385,0.00054157164,0.00034819456,0.0028120994],"category_scores_gemma":[0.0056532566,0.00020652544,0.00050525664,0.00089473923,0.000576844,0.00071908155,0.00078240025,0.0003486174,0.0005488359],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00055281847,0.00008312653,0.9719145,0.000036810772,0.00037890047,0.00016760838,0.000122013764,0.012436512,0.0048459843,0.002887372,0.0005475735,0.0060268715],"study_design_scores_gemma":[0.00002748265,0.000081336446,0.9411128,0.000010167254,0.000051713017,0.00008578862,0.00012477874,0.053075608,0.003300977,0.0014641335,0.00064751745,0.000017705106],"about_ca_topic_score_codex":0.0035817283,"about_ca_topic_score_gemma":0.0028895317,"teacher_disagreement_score":0.0035817283,"about_ca_system_score_codex":0.00026920543,"about_ca_system_score_gemma":0.000121837664,"threshold_uncertainty_score":0.0094073415},"labels":[],"label_agreement":null},{"id":"W4404402337","doi":"10.3847/1538-4357/ad84ba","title":"WALLABY Pilot Survey: Gas-rich Galaxy Scaling Relations from Marginally Resolved Kinematic Models","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; Government of Western Australia; Australian Research Council; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Centre National d’Etudes Spatiales; Bundesministerium für Bildung und Forschung; Science and Industry Endowment Fund","keywords":"Physics; Astrophysics; Galaxy; Kinematics; Scaling; Baryon; Stellar mass; Dark matter; Galaxy formation and evolution; Sky; Astronomy; Star formation; Geometry; Classical mechanics","score_opus":0.019564049116395674,"score_gpt":0.22981018403371137,"score_spread":0.2102461349173157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404402337","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9904945,0.00012430112,0.005849721,0.0000818623,0.0000024455585,0.000028551545,0.0014605195,0.00008946732,0.0018685309],"genre_scores_gemma":[0.99527305,0.00007169331,0.0023794526,0.00002503241,0.0000066179214,0.000037263588,0.00196573,0.0000329717,0.00020823182],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9995534,0.00014840726,0.000019191219,0.00012173306,0.00008748299,0.000069764756],"domain_scores_gemma":[0.99832004,0.000432429,0.00054745766,0.00041952022,0.00013340879,0.00014718149],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013563798,0.0004244017,0.00042581314,0.0009985389,0.00042657083,0.0010142036,0.00067176396,0.00017581327,0.0012613577],"category_scores_gemma":[0.0041272934,0.00027450308,0.0003879938,0.0009250653,0.0005210122,0.00077001064,0.001289238,0.0003109495,0.00027325234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016278244,0.000032006752,0.94563043,0.000040901785,0.00014960139,0.00016503522,0.0006141421,0.030400008,0.0018482195,0.005139734,0.00207195,0.013745135],"study_design_scores_gemma":[0.00003223773,0.000058354177,0.8158735,0.000038923677,0.000039541086,0.00010747653,0.00034767776,0.17447802,0.00089025206,0.005488925,0.0026099547,0.000035149893],"about_ca_topic_score_codex":0.042608388,"about_ca_topic_score_gemma":0.029508542,"teacher_disagreement_score":0.042608388,"about_ca_system_score_codex":0.0007596988,"about_ca_system_score_gemma":0.00043465602,"threshold_uncertainty_score":0.08472073},"labels":[],"label_agreement":null},{"id":"W4404406939","doi":"10.3847/1538-4357/add0b6","title":"The NANOGrav 12.5 yr Data Set: Probing Interstellar Turbulence and Precision Pulsar Timing with PSR J1903+0327","year":2025,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Naval Research; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Goddard Space Flight Center; Eötvös Loránd Tudományegyetem; Canadian Institute for Advanced Research; University of Toronto; National Aeronautics and Space Administration; National Science Foundation","keywords":"Pulsar; Physics; Astronomy; Astrophysics; Interstellar medium; Turbulence; Data set; Galaxy; Computer science; Meteorology","score_opus":0.03652673810274251,"score_gpt":0.34242869481707605,"score_spread":0.3059019567143335,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404406939","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98640114,0.00007308726,0.0013998109,0.00008858457,0.000020095527,0.000023100643,0.009252296,0.0002391738,0.0025027422],"genre_scores_gemma":[0.9686257,0.000056910907,0.0020703305,0.000055107415,0.000025104246,0.00003894434,0.028452022,0.000116157826,0.0005597653],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977714,0.00003556902,0.000016436637,0.000055350258,0.000077629746,0.00003788195],"domain_scores_gemma":[0.9993369,0.00014115653,0.00013024302,0.00021192145,0.00009594959,0.00008390568],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005826209,0.00033281936,0.00041570497,0.0009326475,0.000434667,0.00047860056,0.0006268071,0.00042952795,0.0012978629],"category_scores_gemma":[0.0009869556,0.00017849974,0.0004009719,0.00094777934,0.0003229392,0.00033790048,0.00059812266,0.00043466035,0.0005604295],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019089244,0.00093137595,0.76307195,0.0002220764,0.00054919015,0.0013533307,0.0005320482,0.07254746,0.07868741,0.0039198427,0.021919714,0.05435675],"study_design_scores_gemma":[0.00028199132,0.00030137622,0.86670923,0.000025414967,0.0000895434,0.00053085125,0.00034500452,0.093081266,0.019103931,0.0014524497,0.017996674,0.000082303515],"about_ca_topic_score_codex":0.012043988,"about_ca_topic_score_gemma":0.021394424,"teacher_disagreement_score":0.012043988,"about_ca_system_score_codex":0.00043436087,"about_ca_system_score_gemma":0.00035430325,"threshold_uncertainty_score":0.023947775},"labels":[],"label_agreement":null},{"id":"W4404449909","doi":"10.3847/1538-4357/adb0bc","title":"Polarization Properties of 28 Repeating Fast Radio Burst Sources with CHIME/FRB","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; University of Toronto; Canada Research Chairs; Smithsonian Astrophysical Observatory; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Physics; Pulsar; Astrophysics; Polarization (electrochemistry); Fast radio burst; Galaxy; Binary number; Line-of-sight","score_opus":0.008336575930089466,"score_gpt":0.26267057708102737,"score_spread":0.2543340011509379,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404449909","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977773,0.00014981993,0.0002754273,0.000020831634,0.0000039622323,0.000010915604,0.0008113994,0.000028571283,0.00092182454],"genre_scores_gemma":[0.9966127,0.0000608901,0.00050053006,0.000012892703,0.00001033616,0.000010148021,0.002445707,0.000017243477,0.00032945554],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998061,0.000012452822,0.0000088037095,0.000048701513,0.00006580478,0.000058201036],"domain_scores_gemma":[0.9991504,0.0000970736,0.00028169897,0.000101997466,0.00020831526,0.00016050709],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00034148234,0.0002918975,0.00032118658,0.0018378008,0.0005207875,0.00052334403,0.00035605708,0.00025971406,0.0009619091],"category_scores_gemma":[0.0010151487,0.00019387493,0.00018756658,0.0018814137,0.0002810511,0.0001454817,0.00048013657,0.00021240581,0.00029353454],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003832465,0.00004189585,0.93133616,0.000030371999,0.00009473593,0.00032034193,0.0005001547,0.0003613004,0.04352297,0.0000836821,0.00043006544,0.022895029],"study_design_scores_gemma":[0.000002754381,0.00000976687,0.99885046,0.0000016829184,0.00000813833,0.00008732307,0.000031002663,0.00012240389,0.0005861984,0.000008052111,0.0002883719,0.0000038533076],"about_ca_topic_score_codex":0.038228296,"about_ca_topic_score_gemma":0.056098856,"teacher_disagreement_score":0.038228296,"about_ca_system_score_codex":0.00059652375,"about_ca_system_score_gemma":0.00025919778,"threshold_uncertainty_score":0.0760116},"labels":[],"label_agreement":null},{"id":"W4404531987","doi":"10.3847/1538-4357/ad8133","title":"Holographic Beam Measurements of the Canadian Hydrogen Intensity Mapping Experiment (CHIME)","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Canada Foundation for Innovation; National Science Foundation","keywords":"Physics; Holography; Intensity (physics); Optics; Beam (structure); Astronomy; Astrophysics; Hydrogen","score_opus":0.022683064886385298,"score_gpt":0.227717805466387,"score_spread":0.2050347405800017,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404531987","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8772882,0.00044012154,0.031019606,0.0008072258,0.00011329232,0.0005254841,0.0379699,0.0020012795,0.049834944],"genre_scores_gemma":[0.9407493,0.00017882815,0.038881235,0.00036358472,0.000039637565,0.0002360374,0.013028439,0.0002537403,0.0062691495],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9991991,0.00003838005,0.000007885562,0.00009726525,0.00047422806,0.0001832236],"domain_scores_gemma":[0.99919504,0.000071865186,0.00006235556,0.00013526765,0.00038589773,0.00014963385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081218284,0.0004095337,0.00033422603,0.0010719247,0.0013875029,0.0007077462,0.0008653591,0.00035604095,0.0029236793],"category_scores_gemma":[0.0010268287,0.0003401048,0.00024661323,0.0016335766,0.0006192381,0.0003990314,0.0011776502,0.0007170034,0.00056314527],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":true,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0032495495,0.000590434,0.20740464,0.00032350648,0.00050616194,0.0006912646,0.0017759799,0.008256892,0.52663076,0.0068328734,0.038283236,0.20545462],"study_design_scores_gemma":[0.0002179419,0.00012703724,0.87680835,0.00002085241,0.000077613215,0.00015918593,0.00023942054,0.0080876835,0.08219744,0.000694548,0.031231763,0.00013808344],"about_ca_topic_score_codex":0.3766949,"about_ca_topic_score_gemma":0.67825663,"teacher_disagreement_score":0.6233051,"about_ca_system_score_codex":0.003169129,"about_ca_system_score_gemma":0.0033827235,"threshold_uncertainty_score":0.7490046},"labels":[],"label_agreement":null},{"id":"W4404553327","doi":"10.3847/1538-4357/ad8447","title":"Searching for Emission Lines at z &gt; 11: The Role of Damped Lyα and Hints About the Escape of Ionizing Photons","year":2024,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":36,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; Ministerio de Ciencia e Innovación; National Science Foundation; Royal Society; Danmarks Grundforskningsfond; University of Arizona; National Research Foundation; Science and Technology Facilities Council; European Commission; HORIZON EUROPE European Research Council; Johns Hopkins University; National Aeronautics and Space Administration; UK Research and Innovation","keywords":"Physics","score_opus":0.010689862078195816,"score_gpt":0.2442155961822187,"score_spread":0.2335257341040229,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404553327","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9733487,0.0006821852,0.008762,0.0006274699,0.000029648587,0.000018963192,0.0014758608,0.0010366968,0.014018378],"genre_scores_gemma":[0.99292713,0.00013116463,0.0039589107,0.00014591921,0.000021993055,0.000006157969,0.0009475804,0.00016571926,0.0016953147],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999231,0.000008367582,0.0000033472193,0.000021407426,0.000017813647,0.000026063759],"domain_scores_gemma":[0.9994611,0.00006980742,0.00017554457,0.0000626471,0.00006582425,0.00016519455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038026262,0.00039490397,0.00022795307,0.00096090516,0.00039721403,0.0010180236,0.0005181424,0.0004239551,0.0055591622],"category_scores_gemma":[0.0005532022,0.00026475103,0.00019682154,0.0005408961,0.0002739347,0.0005650376,0.0004009937,0.0005932378,0.0019954701],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072308205,0.00013057754,0.78537637,0.00015907851,0.00012911965,0.0005961205,0.000818971,0.0022875115,0.14457297,0.0035186475,0.007775292,0.05391225],"study_design_scores_gemma":[0.00004831152,0.000086259235,0.95592076,0.0000474976,0.00007686431,0.00033651644,0.00040457238,0.008572807,0.020559281,0.0020719203,0.011837367,0.000037838396],"about_ca_topic_score_codex":0.0022498684,"about_ca_topic_score_gemma":0.0046744226,"teacher_disagreement_score":0.0055591622,"about_ca_system_score_codex":0.00037672388,"about_ca_system_score_gemma":0.0001408264,"threshold_uncertainty_score":0.018597305},"labels":[],"label_agreement":null},{"id":"W4404569850","doi":"10.3847/1538-4357/ad9b91","title":"Impacts and Statistical Mitigation of Missing Data on the 21 cm Power Spectrum: A Case Study with the Hydrogen Epoch of Reionization Array","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Mitacs; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; European Commission; Gordon and Betty Moore Foundation; McGill University; Canadian Institute for Advanced Research; National Research Foundation; Massachusetts Institute of Technology; National Science Foundation","keywords":"Physics; Reionization; Inpainting; Ringing; Spectral density; Estimator; Missing data; Astrophysics; Redshift; Galaxy; Statistics; Computer science; Filter (signal processing); Artificial intelligence; Image (mathematics); Telecommunications; Machine learning","score_opus":0.011991419849893933,"score_gpt":0.2592912550959726,"score_spread":0.24729983524607868,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404569850","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8250358,0.00050059013,0.16878502,0.0011200422,0.000076831624,0.000058238926,0.0003013334,0.00037584503,0.0037463536],"genre_scores_gemma":[0.978017,0.000060028804,0.021297963,0.000041755422,0.000021990974,0.000011799153,0.00007418961,0.000032506257,0.00044280535],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992847,0.00031810362,0.00002471422,0.00008663688,0.00021236617,0.000073520685],"domain_scores_gemma":[0.9861974,0.011181327,0.0007297762,0.000882589,0.0007469171,0.00026203034],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029796555,0.00039145714,0.00046040944,0.0004979399,0.0004975593,0.000820451,0.0008972372,0.00089403236,0.0007944794],"category_scores_gemma":[0.011196641,0.00019194234,0.0003543009,0.00048423733,0.00097524544,0.00065236655,0.00070212554,0.00081370067,0.00009731156],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049030344,0.00018073311,0.021629062,0.00020554921,0.000089210196,0.002874211,0.000450937,0.91784877,0.01620253,0.010212343,0.0017064982,0.028109914],"study_design_scores_gemma":[0.000039636838,0.0002122452,0.009750509,0.000021704223,0.000028532086,0.0005855038,0.00021355723,0.97359866,0.009544492,0.004616601,0.0013540435,0.000034635952],"about_ca_topic_score_codex":0.0043292055,"about_ca_topic_score_gemma":0.0033588714,"teacher_disagreement_score":0.0043292055,"about_ca_system_score_codex":0.00057779864,"about_ca_system_score_gemma":0.00039985313,"threshold_uncertainty_score":0.015758097},"labels":[],"label_agreement":null},{"id":"W4404599481","doi":"10.3847/1538-4357/ad8448","title":"The Extremely Metal-poor SN 2023ufx: A Local Analog to High-redshift Type II Supernovae","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Division of Astronomical Sciences; Science Mission Directorate; Leibniz-Institut für Astrophysik Potsdam; Eötvös Loránd Tudományegyetem; Stockholms Universitet; Science and Technology Facilities Council; Aarhus Universitet; Turun Yliopisto; Universitetet i Oslo; National Science Foundation; University of Minnesota; UK Research and Innovation; Australian Research Council; Space Telescope Science Institute; Nuclear Safety and Security Commission; Háskóli Íslands; Durham University; Istituto Nazionale di Astrofisica; Smithsonian Astrophysical Observatory; Arizona Board of Regents; European Research Council; Gordon and Betty Moore Foundation; Queen's University Belfast; Ohio State University; UK Space Agency; Leibniz-Gemeinschaft; University of Notre Dame; Queen's University; Los Alamos National Laboratory; Johns Hopkins University; Max-Planck-Institut für Astronomie; Ohio Board of Regents; National Central University; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Physics; Supernova; Astrophysics; Redshift; Astronomy; Type (biology); Metal; Galaxy","score_opus":0.013184136278354146,"score_gpt":0.2420431767071142,"score_spread":0.22885904042876004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404599481","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99713707,0.0001535606,0.00030522252,0.000023405468,0.0000060246807,0.0000072666394,0.00020687064,0.000032610544,0.0021279783],"genre_scores_gemma":[0.99874794,0.000051005984,0.00019338162,0.000041524836,0.000009461821,0.000004112429,0.00037665377,0.0000068058,0.000569072],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999398,0.0000071796326,0.0000034252257,0.000016248981,0.000013486535,0.000019785335],"domain_scores_gemma":[0.9998667,0.000009821066,0.00003837593,0.000014526087,0.000010639216,0.000059982005],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000972751,0.00024225964,0.00021997979,0.00044631198,0.00043086935,0.00039691504,0.00016543116,0.00025050493,0.002299434],"category_scores_gemma":[0.00013437991,0.00007716156,0.00015479805,0.00034943628,0.00025726852,0.00016217797,0.00039603456,0.00017336586,0.00042487832],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001066119,0.00021247938,0.8617708,0.00009729983,0.000086459666,0.008590337,0.0006549706,0.00031609455,0.09012037,0.0011627609,0.0026905343,0.033231698],"study_design_scores_gemma":[0.00001452471,0.00020381692,0.97948784,0.000014186811,0.000014963667,0.009371091,0.0002913382,0.00031582505,0.004955118,0.0003541704,0.0049687233,0.000008361714],"about_ca_topic_score_codex":0.0022999549,"about_ca_topic_score_gemma":0.0037600067,"teacher_disagreement_score":0.0022999549,"about_ca_system_score_codex":0.00017606224,"about_ca_system_score_gemma":0.0000732714,"threshold_uncertainty_score":0.007692337},"labels":[],"label_agreement":null},{"id":"W4404601367","doi":"10.3847/1538-4357/ad8916","title":"The SPT-Chandra BCG Spectroscopic Survey. I. Evolution of the Entropy Threshold for ICM Cooling and AGN Feedback in Galaxy Clusters over the Last 10 Gyr","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo; Université de Montréal","funders":"Science and Technology Facilities Council; U.S. Department of Energy; Argonne National Laboratory; National Science Foundation; NASA Headquarters; Space Telescope Science Institute; Office of Science; National Aeronautics and Space Administration; Fermilab; Smithsonian Astrophysical Observatory; University of Chicago; Smithsonian Institution","keywords":"Physics; Astrophysics; Redshift; Active galactic nucleus; Star formation; Galaxy; Galaxy cluster; Astronomy; Radio galaxy; Population","score_opus":0.008066043160049772,"score_gpt":0.2255015700108763,"score_spread":0.21743552685082654,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404601367","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981927,0.00009726213,0.000047973524,0.000021332346,0.000001788305,0.0000020865934,0.0013603658,0.000009112169,0.00026740597],"genre_scores_gemma":[0.99843544,0.000034545035,0.000049256352,0.000006854469,0.0000034277364,0.000001646303,0.0013307793,0.0000025657675,0.0001355062],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983835,0.000020938287,0.000009621564,0.000052252377,0.00003070889,0.000047985886],"domain_scores_gemma":[0.9989172,0.000078809055,0.0005097371,0.00009514341,0.00010532792,0.00029370835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032403928,0.0001590368,0.00018606604,0.0011916289,0.00024282458,0.00041414416,0.00024289174,0.00018780459,0.0011550676],"category_scores_gemma":[0.00082731055,0.00012494397,0.00022943997,0.0006495676,0.00020498852,0.00032057843,0.00048594657,0.00023701257,0.00044116462],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000040122373,0.000009390968,0.9974976,0.0000048899847,0.000021750424,0.000020640508,0.000069985545,0.00005618398,0.0009606677,0.000024569414,0.00013212286,0.0011620057],"study_design_scores_gemma":[4.539066e-7,0.0000074723407,0.999796,7.464174e-7,0.000002594779,0.000019070756,0.000019207779,0.000046161425,0.000044077293,0.0000032085707,0.00006072413,4.7823596e-7],"about_ca_topic_score_codex":0.00829234,"about_ca_topic_score_gemma":0.012776407,"teacher_disagreement_score":0.00829234,"about_ca_system_score_codex":0.00021228414,"about_ca_system_score_gemma":0.00013312366,"threshold_uncertainty_score":0.016488135},"labels":[],"label_agreement":null},{"id":"W4404617294","doi":"10.3847/1538-4357/ad6f03","title":"Puffy Venuses: The Mass–Radius Impact of Carbon-rich Atmospheres on Lava Worlds","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Government of Ontario","keywords":"Exoplanet; Physics; Astrobiology; Atmosphere (unit); Planet; Astrophysics; Thermodynamics","score_opus":0.01030611324948451,"score_gpt":0.24974704033151734,"score_spread":0.23944092708203282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404617294","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943657,0.0001524148,0.00095730805,0.0002398594,0.0000051204956,0.000003343936,0.00008776684,0.000048785452,0.0041398006],"genre_scores_gemma":[0.99970764,0.000016833856,0.00008122899,0.000008400051,0.0000026683358,5.573934e-7,0.000019088486,0.000004557035,0.0001589507],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989414,0.000023074075,0.0000028623913,0.000022225511,0.00002389095,0.000033814347],"domain_scores_gemma":[0.99928385,0.00017470283,0.00018809167,0.00008240415,0.000033724486,0.00023729804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024160798,0.00025033063,0.00018215651,0.00036428362,0.0005210859,0.0011365879,0.00040164505,0.0004929392,0.0027608238],"category_scores_gemma":[0.0011007938,0.000132802,0.0002403551,0.00016473744,0.0008315508,0.0007662764,0.0010173939,0.0002754789,0.00018993678],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011476397,0.00012754196,0.6507154,0.00016298622,0.00030006527,0.0028687217,0.0009998246,0.06558105,0.15821482,0.09083812,0.0032207412,0.025823083],"study_design_scores_gemma":[0.00006454774,0.0003516843,0.6916291,0.000037738402,0.000094321666,0.0015697986,0.0012416993,0.24198182,0.017215967,0.036608655,0.009112567,0.00009213574],"about_ca_topic_score_codex":0.0029359092,"about_ca_topic_score_gemma":0.0016769144,"teacher_disagreement_score":0.0029359092,"about_ca_system_score_codex":0.0005819918,"about_ca_system_score_gemma":0.00016038654,"threshold_uncertainty_score":0.009235859},"labels":[],"label_agreement":null},{"id":"W4404617950","doi":"10.3847/1538-4357/ad808e","title":"A Search for Persistent Radio Sources toward Repeating Fast Radio Bursts Discovered by CHIME/FRB","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"U.S. Naval Research Laboratory; Office of Naval Research; Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Smithsonian Astrophysical Observatory; Science and Technology Facilities Council; University of Toronto; Space Telescope Science Institute; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Fonds de recherche du Québec – Nature et technologies; National Radio Astronomy Observatory; Comisión Nacional de Investigación Científica y Tecnológica; McGill University; Canadian Institute for Advanced Research; Canada Research Chairs; National Aeronautics and Space Administration; Nuclear Safety and Security Commission; Vetenskapsrådet; NASA Headquarters; Ministério da Ciência e Tecnologia; National Science Foundation","keywords":"Physics; Astronomy; Fast radio burst; Astrophysics; Radio astronomy; Neutron star","score_opus":0.01700539544892809,"score_gpt":0.31047811340371734,"score_spread":0.29347271795478924,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404617950","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976042,0.0001963083,0.00073698757,0.000042979722,0.000004613626,0.000017424865,0.00039042896,0.000081878134,0.00092528295],"genre_scores_gemma":[0.9979213,0.000057807316,0.0010873296,0.000043039614,0.000010147517,0.000008170409,0.0005692301,0.0000138283285,0.0002891849],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99975103,0.000016343487,0.000010140453,0.00010025435,0.00005405769,0.00006813204],"domain_scores_gemma":[0.9985862,0.00014486338,0.0006235047,0.0001573982,0.00014304575,0.0003449861],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041125764,0.00030774338,0.00034484974,0.0019121733,0.00051452656,0.00054248114,0.0004071289,0.00028599962,0.0015795721],"category_scores_gemma":[0.0007099772,0.00022428331,0.00032151502,0.0008583876,0.00034289685,0.00020543564,0.00066076417,0.00033393456,0.0004867945],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014976437,0.00003958276,0.95041287,0.000050355546,0.00011090457,0.0006354793,0.0002973442,0.00021260833,0.03413453,0.00011305196,0.00047076555,0.013372836],"study_design_scores_gemma":[0.000005900122,0.000047079207,0.99699795,0.0000079011625,0.000030818526,0.0003684065,0.00016055832,0.00038407787,0.001209281,0.00004387353,0.00073785614,0.0000063441994],"about_ca_topic_score_codex":0.0051580225,"about_ca_topic_score_gemma":0.009053386,"teacher_disagreement_score":0.0051580225,"about_ca_system_score_codex":0.00025077353,"about_ca_system_score_gemma":0.00020853705,"threshold_uncertainty_score":0.010256052},"labels":[],"label_agreement":null},{"id":"W4404704785","doi":"10.3847/1538-4357/ad863b","title":"JWST Resolves Collision-induced Absorption Features in White Dwarfs","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Aeronautics and Space Administration; Canadian Space Agency; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Infrared; White dwarf; Stars; Infrared spectroscopy; Spectrograph; Absorption (acoustics); Spectral line; Astronomy; Optics","score_opus":0.011108326160194169,"score_gpt":0.24445654625844798,"score_spread":0.23334822009825382,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404704785","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982539,0.000068942696,0.0006402409,0.000013103558,0.0000043893347,0.0000030789633,0.00015494852,0.00008461942,0.00077686156],"genre_scores_gemma":[0.9985751,0.00001851951,0.00075342326,0.000016413493,0.0000063195043,0.000002242818,0.00033876862,0.000011501931,0.00027766617],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993587,0.0000030923238,0.000003620662,0.000021019241,0.000018302475,0.00001814126],"domain_scores_gemma":[0.9998184,0.000012856266,0.000044822224,0.000020908377,0.000027951326,0.00007505021],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013229644,0.0001843244,0.00019357313,0.0006141218,0.00024626736,0.00036276103,0.00019663811,0.00018933178,0.0009667253],"category_scores_gemma":[0.00021798273,0.00013245763,0.00014082466,0.0003529608,0.00011925761,0.00020335018,0.00042750448,0.00017361266,0.00032358637],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002766678,0.0000736015,0.5986593,0.000050994237,0.000050255665,0.0004807612,0.00037453684,0.00041237773,0.38445434,0.0002528483,0.000814975,0.014099412],"study_design_scores_gemma":[0.000011052496,0.00007028253,0.98147136,0.0000060878046,0.000021488911,0.00031276516,0.00024823536,0.0017535462,0.0144937895,0.00015050797,0.0014541784,0.0000066351386],"about_ca_topic_score_codex":0.0020870485,"about_ca_topic_score_gemma":0.0053286254,"teacher_disagreement_score":0.0020870485,"about_ca_system_score_codex":0.0001683857,"about_ca_system_score_gemma":0.000096154115,"threshold_uncertainty_score":0.0041497946},"labels":[],"label_agreement":null},{"id":"W4404732482","doi":"10.3847/1538-4357/ad83d5","title":"Impacting Atmospheres: How Late-stage Pollution Alters Exoplanet Composition","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Exoplanet; Physics; Astrobiology; Atmospheric composition; Pollution; Stage (stratigraphy); Light pollution; Astronomy; Atmosphere (unit); Atmospheric sciences; Planet; Meteorology","score_opus":0.01200383524558638,"score_gpt":0.23488481614361045,"score_spread":0.22288098089802408,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404732482","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99774665,0.00010317014,0.0010340902,0.000109615714,0.000005394183,0.000003334199,0.00016080705,0.000028201894,0.00080881384],"genre_scores_gemma":[0.99935335,0.00006397622,0.00018898168,0.000016814061,0.0000016745274,0.000002186386,0.0000769369,0.000011599329,0.00028443141],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999026,0.000020703495,0.000004296372,0.0000382658,0.000011973446,0.000022240522],"domain_scores_gemma":[0.9997652,0.00007621073,0.000055261153,0.000029577866,0.000023073433,0.000050565224],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017431249,0.0003049934,0.00031373277,0.00020476505,0.0003123075,0.0009957721,0.0006458678,0.000830589,0.0021585268],"category_scores_gemma":[0.00069300615,0.00023292677,0.00043193653,0.00021332786,0.00043643088,0.0007340323,0.00053021737,0.00040156275,0.00019387346],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006911322,0.00033488483,0.2729049,0.00018011422,0.00036154728,0.0010374935,0.00056422665,0.45129722,0.25835168,0.0053540906,0.0009873513,0.007935486],"study_design_scores_gemma":[0.0000636974,0.00037125943,0.19790356,0.00001923283,0.00009543592,0.00028953972,0.00066013256,0.7680005,0.026106346,0.0042321817,0.0021887028,0.00006952214],"about_ca_topic_score_codex":0.0057184463,"about_ca_topic_score_gemma":0.0025466103,"teacher_disagreement_score":0.0057184463,"about_ca_system_score_codex":0.0006528896,"about_ca_system_score_gemma":0.00015290723,"threshold_uncertainty_score":0.011370301},"labels":[],"label_agreement":null},{"id":"W4404778755","doi":"10.3847/1538-4357/ad85dd","title":"Eridanus III and DELVE 1: Carbon-rich Primordial Star Clusters or the Smallest Dwarf Galaxies?*","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Vetenskapsrådet; Science and Technology Facilities Council; National Science Foundation","keywords":"Physics; Astrophysics; Astronomy; Dwarf galaxy; Galaxy; Star cluster; Star (game theory); Carbon star; Stars","score_opus":0.012366835467534221,"score_gpt":0.22661088348958117,"score_spread":0.21424404802204694,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404778755","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997832,0.0002683279,0.000100403064,0.000028081005,0.000003754729,0.0000024450692,0.000089858106,0.000006670549,0.0016685091],"genre_scores_gemma":[0.99874204,0.000116241325,0.00028858765,0.000032604683,0.00000438369,0.000001957115,0.0002828375,0.0000029796597,0.00052821875],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991107,0.0000051667203,0.0000035843339,0.0000349708,0.000014273651,0.00003093057],"domain_scores_gemma":[0.999778,0.00002315264,0.000078104924,0.00002640904,0.000021609796,0.00007281721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014508108,0.00012878526,0.0002774513,0.00043295906,0.00023648098,0.0004997355,0.000310878,0.00016302093,0.0009089537],"category_scores_gemma":[0.00026172926,0.00007982891,0.00006317507,0.00021394792,0.00031910502,0.00032477317,0.00038147406,0.00013134479,0.00014146772],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032142553,0.000050601702,0.9477639,0.000070753886,0.000042159118,0.00031838642,0.0003465265,0.00017863957,0.027044775,0.0017011958,0.00052100816,0.021640688],"study_design_scores_gemma":[0.000012060173,0.000056870438,0.9869751,0.000013349382,0.000011833475,0.00052299025,0.00037577486,0.00026723524,0.0035107955,0.00050475023,0.007743306,0.000005953713],"about_ca_topic_score_codex":0.0014930108,"about_ca_topic_score_gemma":0.004607466,"teacher_disagreement_score":0.0014930108,"about_ca_system_score_codex":0.00032047572,"about_ca_system_score_gemma":0.000103189464,"threshold_uncertainty_score":0.003040731},"labels":[],"label_agreement":null},{"id":"W4404778813","doi":"10.3847/1538-4357/ad8912","title":"The Magnetic Field in Quiescent Star-forming Filament G16.96+0.27","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"National Key Research and Development Program of China; National Research Foundation; Science and Technology Facilities Council; Ministry of Science and ICT, South Korea; National Research Foundation of Korea; CAS-SAFEA International Partnership Program for Creative Research Teams; Korea Astronomy and Space Science Institute; Japan Society for the Promotion of Science; Academy of Finland; National Natural Science Foundation of China; Chinese Academy of Sciences; Natural Science Foundation of Shanghai; Royal Society; Shanghai Rising-Star Program","keywords":"Physics; Protein filament; Magnetic field; Star (game theory); Astrophysics; Astronomy; Field (mathematics)","score_opus":0.00794168786255117,"score_gpt":0.23989530118592878,"score_spread":0.2319536133233776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404778813","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989767,0.000040713523,0.00004930924,0.0000118954995,0.0000018846416,0.0000018765693,0.00028038534,0.000015329386,0.0006219208],"genre_scores_gemma":[0.9992773,0.000026410667,0.000107927226,0.000007820108,0.0000034461596,0.0000015408726,0.00043938056,0.000004976759,0.00013126608],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996483,0.0000021372405,0.0000018047697,0.0000113736905,0.0000063048965,0.00001354538],"domain_scores_gemma":[0.9998622,0.000007881425,0.00004632307,0.000013922802,0.000013348679,0.00005627459],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006903837,0.00021000378,0.00021389,0.000459838,0.00026172402,0.00035707562,0.00040762732,0.00017548737,0.0009829215],"category_scores_gemma":[0.00014671094,0.00011282255,0.0001279639,0.000364189,0.00024531453,0.000106715444,0.00030363415,0.00022733146,0.0002672399],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00123361,0.00017674766,0.68739533,0.00007084968,0.00013160125,0.0009957695,0.0003850875,0.0033098576,0.29308403,0.00062364555,0.0010383194,0.011555298],"study_design_scores_gemma":[0.000056875197,0.000075758966,0.992295,0.000007835528,0.000024770467,0.00017542302,0.00008872744,0.0022222546,0.0040617115,0.00016401449,0.00081947126,0.000008055625],"about_ca_topic_score_codex":0.0058484194,"about_ca_topic_score_gemma":0.0050352844,"teacher_disagreement_score":0.0058484194,"about_ca_system_score_codex":0.00038569278,"about_ca_system_score_gemma":0.00010572405,"threshold_uncertainty_score":0.011628747},"labels":[],"label_agreement":null},{"id":"W4404856258","doi":"10.3847/1538-4357/ad88ed","title":"The JCMT BISTRO Survey: The Magnetic Fields of the IC 348 Star-forming Region","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Ministry of Science and ICT, South Korea; National Astronomical Observatory of Japan; Ministry of Science and Technology, Taiwan; National Research Foundation of Korea; Seoul National University; Academia Sinica; National Natural Science Foundation of China; Science and Technology Facilities Council; National Research Foundation; Ministerio de Ciencia e Innovación; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Astronomical Research Institute of Thailand; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; James Clerk Maxwell Telescope; Star (game theory); Astronomy; Star formation; Astrophysics; Stars","score_opus":0.014579256507746911,"score_gpt":0.24020966146255426,"score_spread":0.22563040495480735,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404856258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99765635,0.00006620064,0.00009483845,0.000028482917,0.0000023397288,0.0000062500735,0.0011041125,0.000043835185,0.0009975291],"genre_scores_gemma":[0.9968843,0.000050909155,0.0002766781,0.000022330314,0.000014322319,0.0000066058224,0.0024877863,0.000010397175,0.00024668738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999877,0.000011370089,0.0000056753124,0.000030453075,0.00003967586,0.000035767833],"domain_scores_gemma":[0.99958354,0.000027027423,0.00016020268,0.00004365482,0.000078060475,0.00010759388],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014396978,0.0002236474,0.00018162337,0.0021412536,0.00026979716,0.00025624182,0.00025556696,0.00019585613,0.00078746554],"category_scores_gemma":[0.000409482,0.000117166666,0.00012390132,0.0010617276,0.000139598,0.00014712295,0.00039000856,0.000168637,0.00022487732],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014740902,0.000049681967,0.9506514,0.0000314777,0.00007280087,0.00032791775,0.00022558864,0.0007590099,0.032362364,0.00013676536,0.0020794391,0.013156098],"study_design_scores_gemma":[0.0000030065546,0.000008017654,0.9984946,0.0000016462075,0.0000063619027,0.00005529661,0.000026726842,0.00031688207,0.00041737143,0.000007925637,0.0006602519,0.0000018032903],"about_ca_topic_score_codex":0.013115739,"about_ca_topic_score_gemma":0.01788388,"teacher_disagreement_score":0.013115739,"about_ca_system_score_codex":0.00035643793,"about_ca_system_score_gemma":0.0001761803,"threshold_uncertainty_score":0.02607876},"labels":[],"label_agreement":null},{"id":"W4404863861","doi":"10.3847/1538-4357/ad8b1e","title":"Testable Predictions of Outside-in Age Gradients in Dwarf Galaxies of All Types","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Ames Research Center; Ministry of Colleges and Universities; Institut Périmètre de physique théorique; National Science Foundation; Government of Canada; National Aeronautics and Space Administration; Space Telescope Science Institute","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Dwarf galaxy","score_opus":0.009813283991741282,"score_gpt":0.22843612387562748,"score_spread":0.2186228398838862,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404863861","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989705,0.000014071472,0.000493969,0.000025101072,0.000002187717,0.000003488249,0.00015146619,0.000015033171,0.00032429298],"genre_scores_gemma":[0.9996917,0.0000032196474,0.000119791956,0.000006094576,0.0000010414307,0.0000017024487,0.00010919254,0.0000033942556,0.000063917134],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997136,0.00006534165,0.000012677607,0.00010684013,0.000038124683,0.00006339983],"domain_scores_gemma":[0.9978752,0.00093813456,0.00040849982,0.00023124019,0.00017750186,0.00036945366],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011886276,0.00027347985,0.0003900625,0.00034667822,0.0004343046,0.0008766071,0.000629326,0.0005484095,0.0016066319],"category_scores_gemma":[0.005898099,0.0002506638,0.00035603467,0.00021615748,0.00055041065,0.0006516513,0.00045312542,0.00034051583,0.00020748565],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040019676,0.00008317987,0.90383786,0.000013857957,0.00007130551,0.00010494764,0.00009858119,0.088286504,0.002963605,0.0015277345,0.0002347737,0.0023773503],"study_design_scores_gemma":[0.00013130414,0.00027800087,0.53876436,0.0000110977,0.00005839826,0.00013765294,0.00034398178,0.45214048,0.004593217,0.002794362,0.00072055415,0.000026616744],"about_ca_topic_score_codex":0.007941528,"about_ca_topic_score_gemma":0.006145246,"teacher_disagreement_score":0.007941528,"about_ca_system_score_codex":0.00052336225,"about_ca_system_score_gemma":0.00025865197,"threshold_uncertainty_score":0.015790582},"labels":[],"label_agreement":null},{"id":"W4404927319","doi":"10.3847/1538-4357/ad84dd","title":"Viscous Transonic Accretion Flows in Kerr Black Hole Geometry","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Indian Space Research Organisation; Canadian Patient Safety Institute","keywords":"Physics; Transonic; Accretion (finance); Accretion disc; Astrophysics; Rotating black hole; Black hole (networking); Astronomy; Classical mechanics; Mechanics; Aerodynamics","score_opus":0.011492325770742568,"score_gpt":0.2446888931672809,"score_spread":0.23319656739653832,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404927319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96521807,0.00031896646,0.024880825,0.00017351023,0.000031655625,0.000040756437,0.00008486849,0.00008359958,0.009167734],"genre_scores_gemma":[0.995745,0.00012779898,0.0025943606,0.000026511734,0.000026617503,0.000012439411,0.000042766085,0.000018822957,0.0014057467],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9998714,0.000041716143,0.0000066981693,0.000019570358,0.000021207816,0.000039395796],"domain_scores_gemma":[0.9995722,0.00008898928,0.00016180032,0.000022507053,0.000057192676,0.00009731465],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003431305,0.0007381021,0.00034172498,0.00081611256,0.00048469822,0.0011513014,0.0005013704,0.00049389916,0.0012485826],"category_scores_gemma":[0.0012958285,0.00023445438,0.00040894578,0.00027058416,0.0010535964,0.00096900796,0.0010080145,0.00035454502,0.00018139285],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00061699137,0.00022205654,0.016097024,0.00015010295,0.00012250485,0.0023691135,0.00066386804,0.5984297,0.0730866,0.29976454,0.0010485701,0.0074289027],"study_design_scores_gemma":[0.00008249924,0.00014515594,0.005954374,0.000014030294,0.00001432978,0.00020531054,0.0001393574,0.96756625,0.0024260215,0.022580823,0.0008394295,0.000032282373],"about_ca_topic_score_codex":0.0035466366,"about_ca_topic_score_gemma":0.0010247895,"teacher_disagreement_score":0.0035466366,"about_ca_system_score_codex":0.0006448434,"about_ca_system_score_gemma":0.00029296393,"threshold_uncertainty_score":0.0070519447},"labels":[],"label_agreement":null},{"id":"W4404931361","doi":"10.3847/1538-4357/ad8b1c","title":"MAGAZ3NE: Massive, Extremely Dusty Galaxies at z ∼ 2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3 &lt; z &lt; 4*","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Science and Technology Facilities Council; Durham University; W. M. Keck Foundation; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Luminous infrared galaxy; Photometry (optics); Stars","score_opus":0.010431212517767841,"score_gpt":0.2287254245643072,"score_spread":0.21829421204653934,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404931361","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9956045,0.00011386576,0.0010721056,0.000072282906,0.000005236007,0.0000028879817,0.0007522953,0.0001319008,0.0022449226],"genre_scores_gemma":[0.99899584,0.0000130003455,0.00027158778,0.00004295877,0.0000032458306,0.0000011914558,0.0002801624,0.000010847879,0.00038114897],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997359,0.000045455337,0.000014433797,0.00008962,0.00006200731,0.00005265861],"domain_scores_gemma":[0.99866855,0.00027884732,0.0005096933,0.00024183026,0.0001300873,0.00017105555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006170098,0.0001624595,0.00017864004,0.0005895815,0.00019159143,0.00061264803,0.0002985556,0.00019184792,0.0033302356],"category_scores_gemma":[0.0017180805,0.0001119486,0.00017970028,0.00037857852,0.00027222803,0.0003225189,0.00050612405,0.00021363482,0.0006855515],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016680808,0.000009467425,0.98679197,0.000013550392,0.000031777217,0.00006756311,0.00009574188,0.0002767901,0.00492564,0.0002431916,0.0007869135,0.006590719],"study_design_scores_gemma":[0.000003796208,0.000009435636,0.9964324,0.0000029607247,0.0000126830355,0.00012988976,0.00008588079,0.0005291984,0.0018560151,0.00013788675,0.0007977903,0.0000019930685],"about_ca_topic_score_codex":0.0041834833,"about_ca_topic_score_gemma":0.007800417,"teacher_disagreement_score":0.0041834833,"about_ca_system_score_codex":0.0002691492,"about_ca_system_score_gemma":0.00010227937,"threshold_uncertainty_score":0.011140704},"labels":[],"label_agreement":null},{"id":"W4404959722","doi":"10.3847/1538-4357/ad8c44","title":"Planet Mass Function around M Stars at 1–10 au: A Plethora of Sub-Earth Mass Objects","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Planet; Physics; Planetary mass; Gravitational microlensing; Jupiter mass; Planetary system; Astronomy; Accretion (finance); Astrophysics; Initial mass function; Astrobiology; Exoplanet; Planetary migration; Minimum mass; Stars; Star formation","score_opus":0.01119908383725325,"score_gpt":0.2187387380481399,"score_spread":0.20753965421088666,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4404959722","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9979619,0.00014939519,0.00060521555,0.000021815818,0.0000014313406,0.0000025310883,0.00025474073,0.00007375102,0.0009292933],"genre_scores_gemma":[0.9991155,0.000031542826,0.0003695282,0.000006137431,0.0000027184267,0.000001827373,0.00031792148,0.000008210362,0.00014646644],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994063,0.0000047317585,0.0000021208807,0.00002661184,0.000010905086,0.000015028738],"domain_scores_gemma":[0.9996643,0.00006623692,0.00012265114,0.00004165313,0.00003192712,0.00007320467],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021304819,0.00020853386,0.00021646685,0.0013644886,0.00034730506,0.0005374144,0.00025354358,0.00022913128,0.001119303],"category_scores_gemma":[0.00039728562,0.000112426584,0.00023657456,0.00063786627,0.00020228927,0.000341069,0.00041461442,0.00020860504,0.00036964493],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000120203986,0.000023134298,0.95790315,0.000021899878,0.00003550581,0.00023848376,0.00021262284,0.0010318586,0.026855191,0.00036808616,0.0003506566,0.012839282],"study_design_scores_gemma":[0.0000017442904,0.000015528896,0.9955224,0.0000027508408,0.000006430293,0.00020533155,0.00004930571,0.0022730439,0.0014341057,0.00012135284,0.00036466293,0.0000034723516],"about_ca_topic_score_codex":0.0010000403,"about_ca_topic_score_gemma":0.0010365399,"teacher_disagreement_score":0.0013644886,"about_ca_system_score_codex":0.0002012742,"about_ca_system_score_gemma":0.000052870895,"threshold_uncertainty_score":0.003744483},"labels":[],"label_agreement":null},{"id":"W4405012127","doi":"10.3847/1538-4357/ad8b4e","title":"The Environments of Green Pea Galaxies. II. The Hα Dot Sample","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Indiana University Bloomington; Office of Science; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Instituto de Astrofísica de Canarias; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; U.S. Department of Energy; Smithsonian Institution; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University; Max-Planck-Institut für Astrophysik","keywords":"Physics; Galaxy; Astrophysics; Astronomy; Sample (material)","score_opus":0.011318768433243571,"score_gpt":0.257213581126451,"score_spread":0.24589481269320743,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405012127","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992872,0.000019763582,0.000037142978,0.000006121579,1.7559628e-7,0.0000020260773,0.0002729033,0.0000033762235,0.00037134445],"genre_scores_gemma":[0.9989543,0.000032841817,0.000075800766,0.000010358054,8.48815e-7,0.000002627061,0.00073405664,0.0000027869683,0.00018631353],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998789,0.000013574113,0.000006327225,0.000040450257,0.000023321543,0.000037339443],"domain_scores_gemma":[0.9994962,0.00006459099,0.00017254334,0.000060963863,0.000051214178,0.00015443574],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011946124,0.0001465749,0.00017419303,0.0014013135,0.00031939658,0.0004726066,0.00020236238,0.0001716383,0.0013557909],"category_scores_gemma":[0.00068443874,0.00009988269,0.00011045223,0.0012511559,0.0004727296,0.0004491831,0.0010161826,0.00013206364,0.00031947365],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006791603,0.000013539103,0.9929866,0.0000074119703,0.000014556996,0.0001326447,0.00066445704,0.0000900688,0.002606661,0.0001079747,0.00008877598,0.0032194124],"study_design_scores_gemma":[0.0000014021921,0.000011893619,0.9991321,0.0000014571414,0.0000020348223,0.00007017961,0.00034790998,0.000054854107,0.00010448588,0.00003165419,0.00024120368,8.93761e-7],"about_ca_topic_score_codex":0.011460928,"about_ca_topic_score_gemma":0.029072762,"teacher_disagreement_score":0.011460928,"about_ca_system_score_codex":0.00028485424,"about_ca_system_score_gemma":0.00012701421,"threshold_uncertainty_score":0.022788465},"labels":[],"label_agreement":null},{"id":"W4405032760","doi":"10.3847/1538-4357/ad991d","title":"An Enigmatic PeVatron in an Area around H <scp>ii</scp> Region G35.6−0.5","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Key Research and Development Program of China; Natural Sciences and Engineering Research Council of Canada; National Research Council of Thailand; National Science and Technology Development Agency; National Natural Science Foundation of China; European Space Agency; National Science Foundation","keywords":"Physics; Astrophysics; Cosmic ray; Observatory; Supernova remnant; Spectral index; Supernova; Molecular cloud; Astronomy; Spectral line; Stars","score_opus":0.010525063626341704,"score_gpt":0.24142462546236595,"score_spread":0.23089956183602425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405032760","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998109,0.000093471426,0.00013472392,0.00008781917,0.0000047760864,0.0000031272555,0.00007772293,0.000014896667,0.0014744594],"genre_scores_gemma":[0.9994784,0.000030383075,0.000106240084,0.000025938723,0.000006143432,0.0000010002839,0.000100259225,0.0000021479186,0.00024948822],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999567,0.0000034234026,0.0000014794714,0.000014183751,0.000008562021,0.000015688833],"domain_scores_gemma":[0.99991024,0.000008448266,0.000030133093,0.000008540584,0.000011813271,0.000030801555],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006747317,0.00009229423,0.000082437866,0.0006112849,0.000465408,0.00036510918,0.00018977659,0.00021581068,0.0018060947],"category_scores_gemma":[0.00013678543,0.00007872189,0.00008792968,0.00037949524,0.0003649202,0.0001574265,0.00035686532,0.00014441126,0.00019597252],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014500953,0.000022744263,0.9481226,0.0000363164,0.000037518483,0.003729511,0.0014539603,0.00011530822,0.025229644,0.00039674682,0.0018739189,0.018836644],"study_design_scores_gemma":[0.0000048070347,0.000040960684,0.9913231,0.000012373191,0.000014484252,0.0032811048,0.0011513309,0.00018332813,0.00075576064,0.000118201635,0.0031103767,0.0000040083387],"about_ca_topic_score_codex":0.011426152,"about_ca_topic_score_gemma":0.018736139,"teacher_disagreement_score":0.011426152,"about_ca_system_score_codex":0.00019733794,"about_ca_system_score_gemma":0.00018350335,"threshold_uncertainty_score":0.022719264},"labels":[],"label_agreement":null},{"id":"W4405122061","doi":"10.3847/1538-4357/ad8c24","title":"Exploring Pulsar Timing Precision: A Comparative Study of Polarization Calibration Methods for NANOGrav Data from the Green Bank Telescope","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Office of Naval Research; University of Toronto; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Eötvös Loránd Tudományegyetem; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; Goddard Space Flight Center; West Virginia University; U.S. Naval Research Laboratory; Vanderbilt University; National Science Foundation","keywords":"Pulsar; Physics; Gravitational wave; Green Bank Telescope; Millisecond pulsar; Calibration; Polarization (electrochemistry); Astrophysics; Telescope; Binary pulsar; Supermassive black hole; Crab Pulsar; Astronomy","score_opus":0.2368767415626069,"score_gpt":0.45720132157910504,"score_spread":0.22032458001649813,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405122061","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95556194,0.00038025485,0.04041221,0.00015743676,0.00003247392,0.000026494887,0.00079600234,0.0004512818,0.002181919],"genre_scores_gemma":[0.98041266,0.000119897406,0.017501496,0.000034623703,0.000024559891,0.00001574915,0.001503431,0.00012215122,0.00026537184],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.998692,0.00042285715,0.00008946036,0.00031625963,0.00040620586,0.000073327756],"domain_scores_gemma":[0.9907251,0.005110134,0.0015498032,0.0012374942,0.001250994,0.00012654826],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004633048,0.00031536294,0.00028482167,0.0011764382,0.00032979817,0.00091680407,0.0005356332,0.00048432988,0.0005923835],"category_scores_gemma":[0.013671116,0.00017659791,0.00039133642,0.0016032257,0.00026518808,0.0008909998,0.0005664283,0.00048466725,0.00028336688],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084989367,0.00022611656,0.5753617,0.00021226521,0.00041802024,0.00025465534,0.0009734511,0.10591513,0.022404917,0.00410405,0.0018285156,0.2874513],"study_design_scores_gemma":[0.0000548553,0.00015774007,0.57257307,0.00008171086,0.00012369381,0.00041118922,0.00045282565,0.39963472,0.019143835,0.0021193547,0.0051615136,0.00008551317],"about_ca_topic_score_codex":0.002531015,"about_ca_topic_score_gemma":0.0028974337,"teacher_disagreement_score":0.004633048,"about_ca_system_score_codex":0.00037512035,"about_ca_system_score_gemma":0.00034892693,"threshold_uncertainty_score":0.024502218},"labels":[],"label_agreement":null},{"id":"W4405195712","doi":"10.3847/1538-4357/ad88e8","title":"Filament Accretion and Fragmentation in the Perseus Molecular Cloud","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Molecular cloud; Protein filament; Astrophysics; Fragmentation (computing); Astronomy; Accretion (finance); Cloud computing; Accretion disc; Stars","score_opus":0.007777727329377786,"score_gpt":0.2521383979635401,"score_spread":0.2443606706341623,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405195712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99951947,0.000052139905,0.00007029895,0.000006233807,4.89407e-7,0.000001290374,0.000048752365,0.00000404101,0.00029727654],"genre_scores_gemma":[0.99983335,0.000018557437,0.00005785045,0.0000031773752,0.0000012536877,6.8293707e-7,0.000054048534,7.2302856e-7,0.000030307494],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.000009854759,0.0000032567323,0.00002351395,0.000014628227,0.000019742789],"domain_scores_gemma":[0.99945813,0.00009913869,0.0002925936,0.000038029506,0.000044322896,0.00006781232],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017609262,0.00016324384,0.000116534226,0.00088571163,0.0002589745,0.0003532146,0.00019145485,0.00011690129,0.00038146987],"category_scores_gemma":[0.0006307377,0.00009498208,0.000080056845,0.0004316922,0.00030986665,0.00022771739,0.0002525308,0.000099191595,0.00006645903],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015589983,0.00002004486,0.9730059,0.000013869329,0.00005805939,0.00040762965,0.00012876226,0.0021472943,0.019839419,0.00026929931,0.00009441682,0.0038594007],"study_design_scores_gemma":[0.000005510955,0.00001924136,0.99486697,0.0000041285143,0.000008318811,0.00014592569,0.00006728472,0.002409133,0.0021697127,0.00015749584,0.00014410543,0.0000022089769],"about_ca_topic_score_codex":0.007745804,"about_ca_topic_score_gemma":0.0060512605,"teacher_disagreement_score":0.007745804,"about_ca_system_score_codex":0.00041059035,"about_ca_system_score_gemma":0.00011131747,"threshold_uncertainty_score":0.015401423},"labels":[],"label_agreement":null},{"id":"W4405259067","doi":"10.3847/1538-4357/ad822a","title":"Complex Kinematics of Nebular Gas in Active Galaxies Centered in Cooling X-Ray Atmospheres","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; California Institute of Technology; W. M. Keck Foundation; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Velocity dispersion; Extragalactic astronomy; Redshift; Cooling flow","score_opus":0.013886648890468369,"score_gpt":0.2386596178253984,"score_spread":0.22477296893493004,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405259067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991585,0.0000849238,0.00010605922,0.000011215613,6.576435e-7,0.0000029860123,0.00008718671,0.000015848287,0.0005326614],"genre_scores_gemma":[0.99918777,0.000045410317,0.00018224666,0.00000643499,0.0000023269877,0.0000030705987,0.00023952103,0.000008591437,0.00032462095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999186,0.000011197182,0.0000033649355,0.000023558172,0.000014509783,0.000028808414],"domain_scores_gemma":[0.9997565,0.000043636857,0.000080624864,0.000013227117,0.000018461911,0.000087590604],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001293519,0.00017963465,0.00019300457,0.0010688453,0.0002669402,0.0008052434,0.0002429408,0.00022328392,0.0012397363],"category_scores_gemma":[0.000327392,0.00021528704,0.0001686994,0.0003874294,0.0003082402,0.00027508364,0.0004477147,0.0001628008,0.00025359992],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001984294,0.000048389527,0.92651975,0.000022149101,0.000070244445,0.00037662522,0.0009952886,0.0018439754,0.06304617,0.0007808479,0.0002474945,0.005850568],"study_design_scores_gemma":[0.000003931236,0.000020236203,0.99807113,0.000002373652,0.0000056771014,0.000063763146,0.00009960095,0.0009549147,0.00042987353,0.000070433256,0.0002743893,0.0000037309183],"about_ca_topic_score_codex":0.009100534,"about_ca_topic_score_gemma":0.008785381,"teacher_disagreement_score":0.009100534,"about_ca_system_score_codex":0.00047308978,"about_ca_system_score_gemma":0.00010352822,"threshold_uncertainty_score":0.018095136},"labels":[],"label_agreement":null},{"id":"W4405336296","doi":"10.3847/1538-4357/ad9024","title":"Visual Orbits of Wolf–Rayet Stars. II. The Orbit of the Nitrogen-rich Wolf–Rayet Binary WR 138 Measured with the CHARA Array","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"HORIZON EUROPE European Research Council; California Institute of Technology; European Commission; Office of the Vice President for Research and Economic Development, University at Buffalo; Embry-Riddle Aeronautical University; Research Corporation for Science Advancement; Science Foundation Ireland; Arizona Space Grant Consortium; W. M. Keck Foundation; Georgia State University; National Aeronautics and Space Administration; National Science Foundation","keywords":"Wolf–Rayet star; Physics; Astrophysics; Orbit (dynamics); Astronomy; Stars; Binary star; Binary number","score_opus":0.010937790348022596,"score_gpt":0.22651442968006158,"score_spread":0.215576639332039,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405336296","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969619,0.000047099737,0.00011377183,0.000009264631,0.000002555646,0.0000049233377,0.00062370213,0.000021023105,0.0022156204],"genre_scores_gemma":[0.99885297,0.000016060038,0.00020192395,0.0000029639205,0.000002780877,0.0000025058118,0.0006089765,0.0000045936135,0.0003072994],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996054,0.0000042366164,0.0000026971932,0.000012869381,0.000008897798,0.000010662073],"domain_scores_gemma":[0.99977905,0.000026306308,0.00006935602,0.000016570719,0.000024369856,0.000084366315],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000088251654,0.00013241949,0.0000884047,0.0009403989,0.00015392083,0.00028103637,0.00011873916,0.00017158169,0.0012422587],"category_scores_gemma":[0.00026706158,0.00007562645,0.00013350134,0.0003213042,0.00012787094,0.00016881766,0.00027429117,0.00016828394,0.0004754816],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008812506,0.00009480075,0.8593351,0.000054602966,0.00006652202,0.00043975064,0.0006340198,0.0013878449,0.11244979,0.00062144705,0.0009527014,0.023082122],"study_design_scores_gemma":[0.000008294261,0.00008534839,0.99549145,0.0000045231563,0.000005605625,0.00022519396,0.00010913092,0.0011093238,0.0021966656,0.000080411395,0.0006792115,0.0000048492525],"about_ca_topic_score_codex":0.001980956,"about_ca_topic_score_gemma":0.002113731,"teacher_disagreement_score":0.001980956,"about_ca_system_score_codex":0.00019384925,"about_ca_system_score_gemma":0.00005573261,"threshold_uncertainty_score":0.004155755},"labels":[],"label_agreement":null},{"id":"W4405382546","doi":"10.3847/1538-4357/ad90b3","title":"Massive Star Cluster Formation with Binaries. I. Evolution of Binary Populations","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Supercomputing Center, Korea Institute of Science and Technology Information; Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Star formation; Star cluster; Molecular cloud; Astronomy; Stars; Cluster (spacecraft); Binary star; Stellar evolution; Binary number; Population; Globular cluster","score_opus":0.01195163538739895,"score_gpt":0.2415816947080572,"score_spread":0.22963005932065825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405382546","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974655,0.00008922269,0.0010284312,0.000052243482,0.00001144736,0.000014322348,0.00017110875,0.00003750532,0.0011301808],"genre_scores_gemma":[0.9988851,0.000042135656,0.0005750579,0.000017930073,0.0000045613347,0.000011217807,0.00015438237,0.000012461858,0.00029726527],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997625,0.00006964432,0.0000102241875,0.000046002817,0.000031045714,0.000080588674],"domain_scores_gemma":[0.9990545,0.00032263098,0.00020570958,0.0000859773,0.00007553609,0.00025575983],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007657716,0.0005487284,0.0006877663,0.0007171339,0.000867654,0.001158286,0.0012503392,0.0009686923,0.0016717042],"category_scores_gemma":[0.0026859997,0.00035281578,0.0007564563,0.0007178874,0.0012104016,0.0008431974,0.001231091,0.00076256966,0.00021557584],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002463621,0.00013847697,0.058434706,0.000039374576,0.000118521115,0.00019160862,0.00008431732,0.9336426,0.0017773741,0.003362817,0.0003331596,0.0016306293],"study_design_scores_gemma":[0.00014457165,0.00021509828,0.01969825,0.000011811636,0.000055357246,0.00008252644,0.00012086167,0.97620606,0.0010593735,0.001911403,0.00046861434,0.00002607483],"about_ca_topic_score_codex":0.017023329,"about_ca_topic_score_gemma":0.007384064,"teacher_disagreement_score":0.017023329,"about_ca_system_score_codex":0.001130172,"about_ca_system_score_gemma":0.0005621993,"threshold_uncertainty_score":0.033848464},"labels":[],"label_agreement":null},{"id":"W4405382795","doi":"10.3847/1538-4357/ad8de7","title":"An Empirical Framework Characterizing the Metallicity and Star-formation History Dependence of X-Ray Binary Population Formation and Emission in Galaxies","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Los Alamos National Laboratory; Brookhaven National Laboratory; York University; Ministério da Ciência, Tecnologia e Inovação; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; Lawrence Berkeley National Laboratory; Astrophysics Division; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Office of Science; Fermilab; Max-Planck-Institut für Astronomie; University of Sussex; Space Telescope Science Institute; Institut de Física d'Altes Energies; Eötvös Loránd Tudományegyetem; Yale University; U.S. Department of Energy; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Nuclear Safety and Security Commission; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Centre National d’Etudes Spatiales; Deutsche Forschungsgemeinschaft; Planetary Science Division; Indian Space Research Organisation; Durham University; National Aeronautics and Space Administration; University College London; Carnegie Mellon University; Gordon and Betty Moore Foundation; Pennsylvania State University; College of Engineering, Michigan State University; Argonne National Laboratory; Goddard Space Flight Center; University of California, Los Angeles; University of Washington; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Integrated Electronics Engineering Center, Binghamton University; Queen's University; Harvard University; Ohio State University; Smithsonian Institution; Financiadora de Estudos e Projetos; University of Pennsylvania; National Central University; Queen's University Belfast; California Institute of Technology; New Mexico State University; University of Portsmouth; Vanderbilt University; Science Mission Directorate; National Science Foundation","keywords":"Physics; Astrophysics; Metallicity; Galaxy; Supernova; Star formation; Stellar population; Astronomy; Luminosity; Population; Stellar mass","score_opus":0.015076340294037144,"score_gpt":0.2510291397585349,"score_spread":0.23595279946449776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405382795","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9427485,0.0003481906,0.053300843,0.00045117256,0.000006205682,0.00003578306,0.0005572173,0.0001702908,0.0023818882],"genre_scores_gemma":[0.9957177,0.0000963838,0.003620261,0.000025658032,0.000013344843,0.000017756875,0.0002532195,0.000019383608,0.00023630401],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9993305,0.0002778699,0.000032254884,0.0001831165,0.00008932253,0.00008689167],"domain_scores_gemma":[0.98875475,0.006726715,0.002078611,0.0011050311,0.0008610671,0.00047387538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0029532954,0.000512118,0.00036020816,0.002148798,0.00046244747,0.0016221397,0.00097278296,0.00078549376,0.0014766179],"category_scores_gemma":[0.019210463,0.00032568694,0.00061196554,0.00094041193,0.0015478241,0.0016277381,0.0010800734,0.0007453206,0.00033047865],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000048750942,0.000085518965,0.8558491,0.000041408257,0.00017640207,0.00015465,0.0004477046,0.10776632,0.002096268,0.016953189,0.0005461227,0.015834669],"study_design_scores_gemma":[0.000010324518,0.00006150555,0.39040613,0.000029854988,0.000040332052,0.0002896462,0.0003028859,0.59019214,0.00054652104,0.016898295,0.0011903477,0.00003206029],"about_ca_topic_score_codex":0.011477715,"about_ca_topic_score_gemma":0.006882464,"teacher_disagreement_score":0.011477715,"about_ca_system_score_codex":0.0011841028,"about_ca_system_score_gemma":0.0004933056,"threshold_uncertainty_score":0.022821784},"labels":[],"label_agreement":null},{"id":"W4405533293","doi":"10.3847/1538-4357/ad8ddc","title":"Detection of the Temperature Dependence of the White Dwarf Mass–Radius Relation with Gravitational Redshifts","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Leibniz-Gemeinschaft; National Astronomical Observatories, Chinese Academy of Sciences; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Leibniz-Institut für Astrophysik Potsdam; New Mexico State University; Nanjing University; Yale University; University of Toronto; École Polytechnique Fédérale de Lausanne; Space Telescope Science Institute; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; European Space Agency; Johns Hopkins University; Harvard University; China National Textile and Apparel Council; National Science Foundation; Yunnan University; California Institute of Technology; Ohio State University; Carnegie Institution of Washington; Smithsonian Astrophysical Observatory; Flatiron Health; Smithsonian Institution","keywords":"Physics; White dwarf; Astrophysics; RADIUS; Surface gravity; Redshift; Gravitational redshift; Astronomy; Black dwarf; Stars; Gravitation; Effective temperature; Radial velocity; Galaxy","score_opus":0.005580714169029583,"score_gpt":0.20199594036700422,"score_spread":0.19641522619797464,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405533293","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9908812,0.0003391763,0.0039572828,0.00007391401,0.000009733067,0.000006976943,0.0014013932,0.00031000562,0.00302021],"genre_scores_gemma":[0.9982584,0.00003072801,0.0008291509,0.000021184691,0.000008044407,0.0000030120186,0.00058332767,0.000025686973,0.0002405184],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99875975,0.00018352314,0.000072095085,0.0005198614,0.00033922395,0.00012557824],"domain_scores_gemma":[0.99376607,0.0014073778,0.002514573,0.0011586418,0.0008460949,0.0003072614],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010996148,0.00028171157,0.00032993467,0.002104247,0.00029884037,0.00076824834,0.0003979091,0.0003956191,0.0013694962],"category_scores_gemma":[0.0043246346,0.0004032166,0.00033259476,0.0015814984,0.0005497838,0.00045080885,0.00064465625,0.0003015481,0.00068319205],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004520413,0.000014691315,0.97806734,0.000016652855,0.000071242604,0.00002471173,0.00007928685,0.0005862859,0.01646292,0.00025391785,0.00029457686,0.0040830527],"study_design_scores_gemma":[0.0000020322207,0.000009291996,0.99666303,0.0000017496582,0.000008609253,0.00004897965,0.000013030676,0.00096972083,0.0018728367,0.00007815685,0.00032902,0.0000035033784],"about_ca_topic_score_codex":0.005122793,"about_ca_topic_score_gemma":0.0076089366,"teacher_disagreement_score":0.005122793,"about_ca_system_score_codex":0.00032447113,"about_ca_system_score_gemma":0.00018326084,"threshold_uncertainty_score":0.010185897},"labels":[],"label_agreement":null},{"id":"W4405552806","doi":"10.3847/1538-4357/ad9021","title":"Molecular Gas Mass Measurements of an Active, Starburst Galaxy at z ≈ 2.6 Using ALMA Observations of the [C i], CO, and Dust Emission","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Key Research and Development Program of China; Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Active galactic nucleus; Cosmic dust","score_opus":0.042129009501835867,"score_gpt":0.2806053063435028,"score_spread":0.2384762968416669,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405552806","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987734,0.0000469837,0.00022064238,0.000009899535,0.0000016562633,0.000005295122,0.00016526203,0.00002069957,0.00075622654],"genre_scores_gemma":[0.9991798,0.000020913125,0.0004247457,0.000010194653,0.0000051659704,0.000003986166,0.00024890562,0.0000031694801,0.00010314604],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998932,0.000008267815,0.000005819403,0.000040958108,0.000029320838,0.000022393784],"domain_scores_gemma":[0.99978596,0.000021359447,0.000056487628,0.000026353697,0.00003734053,0.00007248563],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016258967,0.00023544273,0.00017957317,0.0009300697,0.00036436977,0.0004395912,0.0003460774,0.00030015613,0.0006695358],"category_scores_gemma":[0.00034353606,0.00016820003,0.0001911156,0.00033970023,0.0001821485,0.00028897484,0.00038122266,0.00021932117,0.00024575158],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026886695,0.00008912239,0.82166857,0.000022888828,0.000066242326,0.00026757034,0.0004094898,0.00066387915,0.17075348,0.00017349856,0.00018085698,0.005435596],"study_design_scores_gemma":[0.000007951766,0.000052641866,0.9943593,0.0000024540543,0.000021525739,0.000085766136,0.000066846726,0.0011661113,0.0039349534,0.000027223517,0.00027132378,0.000003885603],"about_ca_topic_score_codex":0.0041496437,"about_ca_topic_score_gemma":0.005918131,"teacher_disagreement_score":0.0041496437,"about_ca_system_score_codex":0.00033819248,"about_ca_system_score_gemma":0.000061645784,"threshold_uncertainty_score":0.008251011},"labels":[],"label_agreement":null},{"id":"W4405555131","doi":"10.3847/1538-4357/ad90aa","title":"Cosmic Censorship in Sgr A* and M87*: Observationally Excluding Naked Singularities","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Naked singularity; Astrophysics; Event horizon; Astronomy; Cosmic censorship hypothesis; Supermassive black hole; Black hole (networking); Galaxy; Gravitational singularity; Event (particle physics); Quantum mechanics","score_opus":0.028764488346546137,"score_gpt":0.2558128016447224,"score_spread":0.2270483132981763,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405555131","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99756527,0.00009426785,0.0007722194,0.00004720656,0.0000025417075,0.0000023138562,0.00008805571,0.000012393741,0.0014158733],"genre_scores_gemma":[0.99960405,0.000024404731,0.00019254275,0.000003989,0.000004622588,5.502041e-7,0.00011996722,0.0000021192855,0.000047642043],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972755,0.00006181845,0.000026303398,0.0000662983,0.00006117188,0.000056807374],"domain_scores_gemma":[0.99492705,0.0011318993,0.0020149518,0.00081114593,0.0002924699,0.00082250335],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00089993456,0.00023272212,0.00046649462,0.0016488198,0.0008315781,0.0012315424,0.00044166535,0.00026779107,0.00084721093],"category_scores_gemma":[0.004913419,0.00011889154,0.0003389867,0.000927681,0.0014039817,0.0007755099,0.0013659605,0.00042991035,0.00012001397],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00048716992,0.000061699946,0.9305352,0.00009591591,0.00014236147,0.0017625886,0.0022880628,0.0026317576,0.0072039543,0.038042758,0.0006721884,0.016076487],"study_design_scores_gemma":[0.00004268874,0.00016788176,0.9489158,0.000052741318,0.00009211847,0.0015556709,0.00141039,0.011161025,0.0025320638,0.03172914,0.0023041768,0.0000363368],"about_ca_topic_score_codex":0.0040873536,"about_ca_topic_score_gemma":0.0047715525,"teacher_disagreement_score":0.0040873536,"about_ca_system_score_codex":0.0003989175,"about_ca_system_score_gemma":0.00030466035,"threshold_uncertainty_score":0.008127153},"labels":[],"label_agreement":null},{"id":"W4405561771","doi":"10.3847/1538-4357/adcd73","title":"<tt>ChronoFlow:</tt> A Data-driven Model for Gyrochronology","year":2025,"lang":"en","type":"preprint","venue":"The Astrophysical Journal","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; University of Toronto; Government of Ontario","keywords":"Computer science","score_opus":0.02624321105206142,"score_gpt":0.2836780105634247,"score_spread":0.2574347995113633,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405561771","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.16891555,0.00035677792,0.79832065,0.001864949,0.00024246756,0.00016766143,0.013878433,0.0041159205,0.012137543],"genre_scores_gemma":[0.83961064,0.00027741055,0.14261545,0.00040971575,0.00012010004,0.00051965174,0.0064828736,0.0010889886,0.0088751195],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996431,0.00009954285,0.000017095806,0.00013634004,0.000059175894,0.000044706365],"domain_scores_gemma":[0.9988024,0.0004283667,0.0001677852,0.0002544581,0.00020527754,0.00014175873],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015669835,0.00076574204,0.0005363119,0.00092913874,0.0007824107,0.0017551065,0.0022565802,0.0012457032,0.006662411],"category_scores_gemma":[0.0050304946,0.0005204188,0.0011341625,0.0009023375,0.0009266726,0.0017080406,0.0012075112,0.0010496181,0.0012668383],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007325319,0.000031138097,0.016526308,0.00003838077,0.00007135177,0.00008306295,0.00013877223,0.9121413,0.00092745124,0.05453988,0.005110206,0.010318885],"study_design_scores_gemma":[0.00001234515,0.000006655893,0.0011926503,0.000009477377,0.000007569172,0.000023015722,0.000010957512,0.97729605,0.00021086773,0.01728858,0.0039273347,0.0000144749565],"about_ca_topic_score_codex":0.041366506,"about_ca_topic_score_gemma":0.03604244,"teacher_disagreement_score":0.041366506,"about_ca_system_score_codex":0.002169763,"about_ca_system_score_gemma":0.0013229223,"threshold_uncertainty_score":0.08225149},"labels":[],"label_agreement":null},{"id":"W4405562086","doi":"10.3847/1538-4357/ada1cf","title":"Fermi Unassociated Sources in the MeerKAT Absorption Line Survey","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Argonne National Laboratory; Planetary Science Division; Science and Technology Facilities Council; Science Mission Directorate; Smithsonian Astrophysical Observatory; Jet Propulsion Laboratory; University of Illinois at Urbana-Champaign; Office of Science; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; Chinese Academy of Sciences; High Energy Physics; Deutsche Forschungsgemeinschaft; Ohio State University; National Research Foundation; Commonwealth Scientific and Industrial Research Organisation; Gordon and Betty Moore Foundation; Queen's University Belfast; Australian Government; Smithsonian Institution; U.S. Department of Energy; National Radio Astronomy Observatory; Space Telescope Science Institute; University of California, Los Angeles; University of Portsmouth; Science and Industry Endowment Fund; Los Alamos National Laboratory; Johns Hopkins University; University of Chicago; SLAC National Accelerator Laboratory; Queen's University; California Institute of Technology; National Central University; University of Sussex; National Aeronautics and Space Administration; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; Government of Western Australia; Financiadora de Estudos e Projetos; University of Pennsylvania; Durham University; National Science Foundation","keywords":"Physics; Pulsar; Fermi Gamma-ray Space Telescope; Astrophysics; Astronomy; Galaxy; Telescope; Radio telescope; Radio spectrum; Redshift; Spitzer Space Telescope; Radio galaxy; Spectral index; Active galactic nucleus; Quasar; Spectral line","score_opus":0.01254004840869587,"score_gpt":0.24888643006961333,"score_spread":0.23634638166091745,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405562086","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9957769,0.00023970759,0.00054534175,0.000029404857,0.0000043282625,0.000012864027,0.0017567613,0.000044730237,0.0015900391],"genre_scores_gemma":[0.9945661,0.000104087856,0.0008319421,0.000027046823,0.000006077865,0.000007646104,0.0036511319,0.000008309033,0.0007976531],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997533,0.000030337744,0.00002156216,0.000058319085,0.00006950342,0.00006699261],"domain_scores_gemma":[0.9989768,0.00015246993,0.00045060588,0.00012669068,0.00014188561,0.0001516043],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004816635,0.00018012775,0.00017692639,0.0027296504,0.00034941628,0.00052924687,0.00027937308,0.000152846,0.0019930368],"category_scores_gemma":[0.00081616314,0.00010729451,0.00015794794,0.0014517627,0.0002047998,0.00029737386,0.00065332063,0.00013531212,0.0006291332],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000113795446,0.00002269268,0.98366874,0.000013556131,0.000028022414,0.000112154885,0.00017286853,0.00012867307,0.0039634816,0.00017613356,0.00063993735,0.010960052],"study_design_scores_gemma":[0.000004644558,0.000022544713,0.9963735,0.00000554984,0.00001593542,0.00013039315,0.00006323219,0.00019989924,0.001380918,0.000049285307,0.0017511836,0.0000030979843],"about_ca_topic_score_codex":0.007993143,"about_ca_topic_score_gemma":0.011491829,"teacher_disagreement_score":0.007993143,"about_ca_system_score_codex":0.00024896036,"about_ca_system_score_gemma":0.00026507658,"threshold_uncertainty_score":0.01589322},"labels":[],"label_agreement":null},{"id":"W4405580201","doi":"10.3847/1538-4357/ad98ed","title":"Are Long Gamma-Ray Bursts Progenitors to Merging Binary Black Holes?","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; LIGO; Population; Redshift; Astrophysics; Binary number; Algorithm; Gravitational wave; Database; Computer science; Galaxy; Medicine","score_opus":0.01318850451583242,"score_gpt":0.2521677591533582,"score_spread":0.23897925463752578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405580201","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99640626,0.00070118497,0.0018590036,0.00007731416,0.000009518292,0.0000059055906,0.000114346636,0.00006184596,0.00076467555],"genre_scores_gemma":[0.99931836,0.00017141123,0.00018349291,0.000017608843,0.000015043296,0.00000179566,0.00012223262,0.000011535427,0.0001585892],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99985266,0.000025895284,0.000013103284,0.000048641075,0.000023246854,0.0000364627],"domain_scores_gemma":[0.9972224,0.00089413277,0.0013110932,0.0001865382,0.00015119508,0.00023454097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00057304284,0.00031572575,0.00033134656,0.0012732659,0.00022065055,0.0016500179,0.00038888364,0.0005708927,0.0025703912],"category_scores_gemma":[0.003863837,0.00027349056,0.00018486475,0.00083135033,0.00048367406,0.00074863626,0.00031697162,0.00023441482,0.000696095],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038822167,0.000038489667,0.954948,0.000064387335,0.00007164626,0.0010597127,0.0003222319,0.0017091483,0.023845987,0.0026789645,0.00034920048,0.01452393],"study_design_scores_gemma":[0.000046935784,0.00011185131,0.95688033,0.00004042129,0.00008079784,0.005101969,0.000666453,0.018152049,0.010580814,0.005766317,0.002537097,0.000034886965],"about_ca_topic_score_codex":0.0012336181,"about_ca_topic_score_gemma":0.00069758686,"teacher_disagreement_score":0.0025703912,"about_ca_system_score_codex":0.00038367638,"about_ca_system_score_gemma":0.00012427382,"threshold_uncertainty_score":0.0085988045},"labels":[],"label_agreement":null},{"id":"W4405593570","doi":"10.3847/1538-4357/ad8ddf","title":"Interpolation Techniques for Reconstructing Galactic Faraday Rotation","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Agencia Estatal de Investigación; European Research Council; Natural Sciences and Engineering Research Council of Canada; Comunidad de Madrid","keywords":"Physics; Faraday effect; Interpolation (computer graphics); Rotation (mathematics); Astronomy; Astrophysics; Classical mechanics; Geometry; Motion (physics); Magnetic field","score_opus":0.012201981895433008,"score_gpt":0.26001423664234935,"score_spread":0.24781225474691634,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405593570","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.41396293,0.00029218808,0.5807896,0.00011862147,0.00003073767,0.000040835832,0.00035847747,0.0019628585,0.0024436768],"genre_scores_gemma":[0.7977497,0.00008351721,0.20117487,0.000013708569,0.000010556652,0.000025958481,0.00037575685,0.00019125249,0.00037472998],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99975187,0.00009784625,0.000012950209,0.00003640409,0.00007352378,0.00002731762],"domain_scores_gemma":[0.9980564,0.0010306246,0.00020280485,0.00028339933,0.00037211837,0.000054525128],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014127843,0.0003631659,0.00030138917,0.0010115076,0.00027716975,0.00044354264,0.0006869438,0.00034793274,0.001122908],"category_scores_gemma":[0.007665932,0.0002827319,0.0004367193,0.00086372596,0.0002597886,0.00045159916,0.00046492094,0.0004978599,0.00032479514],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021730232,0.000054122247,0.016034761,0.000057951183,0.000059846767,0.000049515827,0.00013446121,0.87629205,0.007045368,0.0040596877,0.00046324416,0.09553169],"study_design_scores_gemma":[0.000010718468,0.000014955984,0.0027631961,0.000006549944,0.0000036069262,0.000014194031,0.000014465234,0.9940499,0.0017977399,0.0010087774,0.00030633315,0.0000095876885],"about_ca_topic_score_codex":0.008550626,"about_ca_topic_score_gemma":0.005528937,"teacher_disagreement_score":0.008550626,"about_ca_system_score_codex":0.00039120944,"about_ca_system_score_gemma":0.0005081521,"threshold_uncertainty_score":0.017001688},"labels":[],"label_agreement":null},{"id":"W4405595467","doi":"10.3847/1538-4357/ad90bb","title":"New Radio Observations of the Supernova Remnant CTA 1","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Research Council Canada; Natural Sciences and Engineering Research Council of Canada; Smithsonian Astrophysical Observatory; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Supernova remnant; Astrophysics; Cassiopeia A; Telescope; Stars; Line-of-sight; Faraday effect; Supernova; Polarization (electrochemistry); Astronomy; Magnetic field","score_opus":0.016937047883278454,"score_gpt":0.227459905214588,"score_spread":0.21052285733130954,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405595467","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924367,0.00019758688,0.00058154156,0.00004392933,0.000014251201,0.000014907325,0.00069818745,0.00011583653,0.0058969934],"genre_scores_gemma":[0.9955877,0.00010820778,0.0010766675,0.00003752182,0.000025322688,0.000009868449,0.0020002823,0.000020004632,0.0011344205],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999181,0.000006319633,0.0000035767446,0.000019269997,0.000033896522,0.00001883546],"domain_scores_gemma":[0.9996599,0.000027723383,0.000088897665,0.000034203815,0.000071358154,0.00011792773],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001601202,0.00017487902,0.00021741049,0.0010305174,0.0002935964,0.00044459288,0.00028569056,0.00019086593,0.001834157],"category_scores_gemma":[0.00039824116,0.00016282627,0.0001465412,0.0005568142,0.00014272361,0.00025870325,0.00054633373,0.000450932,0.0004576168],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006564525,0.0001859008,0.41512355,0.00013727466,0.00012929158,0.0037062753,0.0016507016,0.0009393797,0.5390396,0.00090560346,0.0035224303,0.034003507],"study_design_scores_gemma":[0.000015241639,0.00016871367,0.98491424,0.000021202513,0.000027600017,0.0014021959,0.00019491054,0.0008485653,0.0061820457,0.00007781806,0.006129835,0.000017708453],"about_ca_topic_score_codex":0.0025822055,"about_ca_topic_score_gemma":0.006893339,"teacher_disagreement_score":0.0025822055,"about_ca_system_score_codex":0.00018774281,"about_ca_system_score_gemma":0.00010280309,"threshold_uncertainty_score":0.006135881},"labels":[],"label_agreement":null},{"id":"W4405598370","doi":"10.3847/1538-4357/ad9471","title":"Signatures of Massive Black Hole Merger Host Galaxies from Cosmological Simulations. II. Unique Stellar Kinematics in Integral Field Unit Spectroscopy","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs","keywords":"Physics; Astrophysics; Galaxy; Stellar mass; Stellar kinematics; Astronomy; Star formation; Milky Way","score_opus":0.009821310751976868,"score_gpt":0.24481460959869156,"score_spread":0.2349932988467147,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405598370","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99833065,0.000032759308,0.0007831637,0.00003377748,0.0000023649134,0.0000065423014,0.00024252386,0.00007068443,0.0004976124],"genre_scores_gemma":[0.9977157,0.000014921318,0.001559419,0.000013470944,0.0000030398742,0.000005119395,0.0005840746,0.00002487841,0.00007927748],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99991286,0.000026574,0.00000391208,0.000021034719,0.000017188302,0.000018402548],"domain_scores_gemma":[0.99958783,0.00012706894,0.000102860104,0.000054804754,0.000044581622,0.00008293672],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040041807,0.00042482713,0.00023609822,0.000598259,0.00029695962,0.0004638762,0.00052905927,0.00039356676,0.00049963006],"category_scores_gemma":[0.001198818,0.0002510149,0.0005395702,0.00040505585,0.00031526163,0.00029257484,0.00046203,0.00026644737,0.000099312645],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00052883837,0.0002921852,0.35230142,0.00007635129,0.00035649305,0.000268357,0.00022535137,0.60972905,0.020668807,0.0025032735,0.00094901177,0.012100852],"study_design_scores_gemma":[0.00005802581,0.00007154149,0.09421067,0.0000063366447,0.000040554347,0.000059789752,0.000059923044,0.9013395,0.0031196885,0.00060596305,0.00041043662,0.000017493432],"about_ca_topic_score_codex":0.010149532,"about_ca_topic_score_gemma":0.00939212,"teacher_disagreement_score":0.010149532,"about_ca_system_score_codex":0.00053028914,"about_ca_system_score_gemma":0.00024235852,"threshold_uncertainty_score":0.02018094},"labels":[],"label_agreement":null},{"id":"W4405615044","doi":"10.3847/1538-4357/ad8de0","title":"A Search Using GEO600 for Gravitational Waves Coincident with Fast Radio Bursts from SGR 1935+2154","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Direcció General de Recerca, Generalitat de Catalunya; European Social Fund; Japan Society for the Promotion of Science; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; National Science and Technology Council; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, Culture, Sports, Science and Technology; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, India; Agencia Estatal de Investigación; Great Southern Development Commission, Government of Western Australia; Israel Science Foundation; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Istituto Nazionale di Fisica Nucleare; U.S. Department of Energy; National Research, Development and Innovation Office; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Council of Scientific and Industrial Research, India; University of Tokyo; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Leverhulme Trust; European Commission; Russian Science Foundation; Scottish Funding Council; Narodowa Agencja Wymiany Akademickiej; Centres de Recerca de Catalunya; Institut des Origines de Lyon; Fonds De La Recherche Scientifique - FNRS; Ministerio de Ciencia, Innovación y Universidades; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; Magnetar; LIGO; Astrophysics; Fast radio burst; Gravitational wave; Astronomy; Neutron star","score_opus":0.020690181784522255,"score_gpt":0.3352652333830041,"score_spread":0.31457505159848187,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405615044","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99803764,0.000048685386,0.00052588165,0.000023414503,0.0000023546697,0.0000056987988,0.00038574345,0.00001975727,0.00095086836],"genre_scores_gemma":[0.99727136,0.00002119008,0.0009089411,0.000015402195,0.0000049838595,0.0000030409756,0.0014951087,0.0000045107336,0.0002755043],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973756,0.000035731417,0.000017947257,0.00008078635,0.00007774795,0.000050208142],"domain_scores_gemma":[0.99919957,0.00024947093,0.00020943487,0.00008144175,0.00009360649,0.000166499],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041355772,0.00021040365,0.0002066066,0.0017164431,0.0002935046,0.00054937834,0.00030159613,0.0002378937,0.0013593192],"category_scores_gemma":[0.00091461197,0.000112990725,0.00026731964,0.0010840172,0.00018801296,0.00021392202,0.00046150837,0.000108683635,0.0002785518],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045183094,0.000087372835,0.963289,0.000021182574,0.00013665632,0.0006686116,0.00007117635,0.0010852953,0.01806674,0.00034245223,0.0005003564,0.015279349],"study_design_scores_gemma":[0.000024763163,0.0001604594,0.9880916,0.000005665639,0.000072513816,0.0005022236,0.00015913373,0.0057862727,0.0035362835,0.00010914418,0.0015397391,0.000012210047],"about_ca_topic_score_codex":0.011748253,"about_ca_topic_score_gemma":0.016603032,"teacher_disagreement_score":0.011748253,"about_ca_system_score_codex":0.00032156098,"about_ca_system_score_gemma":0.0003294927,"threshold_uncertainty_score":0.023359716},"labels":[],"label_agreement":null},{"id":"W4405618420","doi":"10.3847/1538-4357/ad909f","title":"The Star Clusters as Links between Galaxy Evolution and Star Formation Project. I. Numerical Method","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Key Research and Development Program of China; Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China; National Aeronautics and Space Administration; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Intergalactic star; Star cluster; Star formation; Astrophysics; Star (game theory); Astronomy; Galaxy formation and evolution; Protogalaxy; Galaxy; Galaxy cluster; Galaxy merger","score_opus":0.01440860681753887,"score_gpt":0.27319176320926863,"score_spread":0.2587831563917298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405618420","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1049676,0.00060480624,0.8505021,0.0008841168,0.0003590965,0.00054449047,0.0060461364,0.0037788153,0.03231284],"genre_scores_gemma":[0.4101761,0.000367338,0.5738938,0.00022077758,0.00012310609,0.0012622604,0.0024426864,0.0009828366,0.010531137],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99972683,0.000121678495,0.000017105587,0.00004846364,0.000058718066,0.00002709117],"domain_scores_gemma":[0.99932754,0.00029425469,0.0000862964,0.000120338475,0.00011605541,0.000055594373],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069493207,0.0004477032,0.00044227473,0.0005297624,0.00046368144,0.0011701605,0.0018984355,0.0008689794,0.00541161],"category_scores_gemma":[0.0030785527,0.0003886883,0.0005072438,0.00065477774,0.0005964922,0.0006737348,0.0010148223,0.0008750015,0.001171125],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012362051,0.00011164423,0.007827406,0.00018791704,0.00009457221,0.00016993364,0.00012236195,0.8642376,0.0027931482,0.09379608,0.0063399025,0.02419591],"study_design_scores_gemma":[0.000034685836,0.000008810477,0.00042081546,0.000012018389,0.0000059906183,0.000017082111,0.000014077718,0.98445547,0.00053669605,0.00927138,0.0052151363,0.00000786327],"about_ca_topic_score_codex":0.007902863,"about_ca_topic_score_gemma":0.005393426,"teacher_disagreement_score":0.007902863,"about_ca_system_score_codex":0.00091739255,"about_ca_system_score_gemma":0.001262657,"threshold_uncertainty_score":0.0181036},"labels":[],"label_agreement":null},{"id":"W4405758729","doi":"10.3847/1538-4357/ad932e","title":"The Intrinsic Flattening of Galaxy Disks","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec; Queen's University","funders":"Agencia Estatal de Investigación; Natural Sciences and Engineering Research Council of Canada; Ministerio de Ciencia e Innovación; Queen's University; Canadian Institute for Theoretical Astrophysics","keywords":"Physics; Flattening; Astrophysics; Astronomy; Galaxy; Galaxy formation and evolution","score_opus":0.007160372139847539,"score_gpt":0.2212394266098533,"score_spread":0.21407905447000575,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405758729","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99678195,0.00028603888,0.00067596853,0.000005600807,0.0000016558387,0.000002650794,0.0005909272,0.000034134926,0.0016209775],"genre_scores_gemma":[0.99957246,0.000028293702,0.00010631161,0.0000024937704,0.0000021715734,7.49097e-7,0.00020822586,0.000003213708,0.000075995165],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978334,0.000029705723,0.0000152455905,0.00007409994,0.000054981807,0.00004269982],"domain_scores_gemma":[0.9982116,0.0002844936,0.00051503646,0.00046491477,0.00036688225,0.00015707515],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026219658,0.0002412597,0.0001671842,0.0014538933,0.00022420997,0.0006997145,0.00025258475,0.00017793998,0.0018011729],"category_scores_gemma":[0.0014163967,0.00015307237,0.00014943517,0.00079257117,0.00043425884,0.0004129632,0.00033555113,0.00019714196,0.00038908867],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009941922,0.000009103201,0.9481703,0.000034842164,0.000070384645,0.000073556024,0.00010885576,0.00095204054,0.039792318,0.00023272535,0.000100514146,0.010355982],"study_design_scores_gemma":[5.151246e-7,0.000011715878,0.9968694,0.000002641046,0.0000055548317,0.00010738967,0.000027905236,0.00041349826,0.0022848407,0.000091324444,0.00018250864,0.000002621223],"about_ca_topic_score_codex":0.0026075395,"about_ca_topic_score_gemma":0.0023896396,"teacher_disagreement_score":0.0026075395,"about_ca_system_score_codex":0.0003264638,"about_ca_system_score_gemma":0.0001076219,"threshold_uncertainty_score":0.006025493},"labels":[],"label_agreement":null},{"id":"W4405763679","doi":"10.3847/1538-4357/ad946c","title":"Separating Super-puffs versus Hot Jupiters among Young Puffy Planets","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Hot Jupiter; Planet; Astrophysics; Exoplanet; Astrobiology; Astronomy; Planetary system; Brown dwarf","score_opus":0.01388646707016516,"score_gpt":0.24416107436823398,"score_spread":0.2302746072980688,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405763679","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991757,0.00013085405,0.00021686983,0.000010137856,9.4111147e-7,0.000002718033,0.00011537515,0.000006806274,0.00034048807],"genre_scores_gemma":[0.9996561,0.00003058989,0.00012689983,0.0000027989397,0.0000018951961,0.0000012788622,0.00013923418,0.0000010974308,0.000040122777],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985373,0.00001468673,0.000012508048,0.00005028596,0.00002149419,0.000047317513],"domain_scores_gemma":[0.9990019,0.00028641114,0.00036949126,0.00007717964,0.00007822418,0.00018678053],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025542738,0.0001915487,0.00020668382,0.0018390706,0.000374219,0.0006286369,0.00025714614,0.00026321597,0.0012760741],"category_scores_gemma":[0.0014860294,0.00008413199,0.00016805367,0.0007087904,0.00036910054,0.0005334543,0.00062055653,0.0001567009,0.00030557695],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000108999724,0.000006890407,0.9875351,0.000016123571,0.000019486632,0.00018565948,0.00022063512,0.00017377424,0.0059436457,0.000110623776,0.00008411511,0.0055948757],"study_design_scores_gemma":[0.0000017297923,0.000043150965,0.996191,0.000010944015,0.000013786985,0.00064818026,0.00047972778,0.00085198396,0.0011255255,0.00021361654,0.0004170786,0.0000031897291],"about_ca_topic_score_codex":0.0014636124,"about_ca_topic_score_gemma":0.002410278,"teacher_disagreement_score":0.0018390706,"about_ca_system_score_codex":0.00016377424,"about_ca_system_score_gemma":0.000086543376,"threshold_uncertainty_score":0.0042688847},"labels":[],"label_agreement":null},{"id":"W4405813068","doi":"10.3847/1538-4357/ad8911","title":"Star−Disk Collisions: Implications for Quasi-periodic Eruptions and Other Transients near Supermassive Black Holes","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":33,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Gordon Foundation","keywords":"Physics; Astrophysics; Supermassive black hole; Accretion (finance); Debris disk; Astronomy; Collision; Flare; Black hole (networking); Shock wave; Stellar collision; Debris; Intermediate-mass black hole; Stellar evolution; Stars; Galaxy; Planetary system; Meteorology; Mechanics","score_opus":0.021934851486663076,"score_gpt":0.2781609603708429,"score_spread":0.25622610888417985,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405813068","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99651825,0.00017019766,0.0010478481,0.00015691624,0.000012476739,0.000014607223,0.00019001121,0.00009095587,0.0017987732],"genre_scores_gemma":[0.9989372,0.00007491631,0.0005017314,0.000030012698,0.00001589457,0.000008112579,0.00010887646,0.000026380338,0.00029686146],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997931,0.00004755626,0.000018097928,0.00007219405,0.000030155952,0.000038874674],"domain_scores_gemma":[0.99865925,0.0003957912,0.00046504385,0.00016429843,0.00007251623,0.0002431137],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00052925694,0.00031286388,0.0006544804,0.00078342087,0.0008096737,0.001116405,0.0009670666,0.0007608725,0.002283446],"category_scores_gemma":[0.0018189003,0.00035270484,0.0006225612,0.00075256,0.0006713943,0.0007758322,0.0013515545,0.0004678928,0.00022643156],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00047751988,0.00034098048,0.6711552,0.00014322918,0.00039329263,0.0024916788,0.0007666256,0.27411306,0.026623446,0.010151842,0.0015827913,0.011760365],"study_design_scores_gemma":[0.00013002692,0.000152461,0.43122128,0.000020262498,0.000063908206,0.0005628961,0.0003246635,0.5596268,0.0023922068,0.0040304405,0.001387499,0.00008748922],"about_ca_topic_score_codex":0.010104462,"about_ca_topic_score_gemma":0.0038852587,"teacher_disagreement_score":0.010104462,"about_ca_system_score_codex":0.0013533076,"about_ca_system_score_gemma":0.00034187437,"threshold_uncertainty_score":0.020091295},"labels":[],"label_agreement":null},{"id":"W4405826927","doi":"10.3847/1538-4357/ad99cd","title":"The Globular Cluster System of the Virgo Cluster Ultradiffuse Galaxy VCC 615","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Ministry of Science and ICT, South Korea; Space Telescope Science Institute; National Research Foundation; National Research Foundation of Korea; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Globular cluster; Virgo Cluster; Astrophysics; Cluster (spacecraft); Astronomy; Brightest cluster galaxy; Galaxy; Galaxy cluster; Dwarf galaxy; Star cluster","score_opus":0.00655427420019635,"score_gpt":0.2091546126238166,"score_spread":0.20260033842362024,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405826927","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99648005,0.000110832116,0.00030706124,0.000030157144,0.000003000729,0.0000075314674,0.0004630004,0.00002800752,0.002570404],"genre_scores_gemma":[0.99752706,0.000027647853,0.00050135585,0.00003009096,0.0000025133104,0.0000043785826,0.0014194959,0.000009010104,0.00047846095],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998305,0.000010140264,0.0000050416816,0.000060018854,0.00005034765,0.000044030538],"domain_scores_gemma":[0.999729,0.000024528232,0.00005372014,0.000040935145,0.000042979264,0.000108744964],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018821062,0.00015707714,0.00016928594,0.0011081367,0.000578923,0.00069771847,0.00037143854,0.00021714924,0.0020227567],"category_scores_gemma":[0.0005041338,0.00010767209,0.00017318047,0.0006781814,0.00029718026,0.00023245554,0.00077323196,0.0001426621,0.0003360885],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019124948,0.000055402732,0.9315576,0.00005971567,0.00009122649,0.00038539746,0.00048321535,0.0041983863,0.030379133,0.0048412126,0.0033639916,0.024393525],"study_design_scores_gemma":[0.000008837268,0.000030175923,0.9859482,0.000012801573,0.00001845365,0.00016527023,0.00018166867,0.006169399,0.0020051927,0.0005917482,0.0048558996,0.0000122051915],"about_ca_topic_score_codex":0.021922853,"about_ca_topic_score_gemma":0.021899812,"teacher_disagreement_score":0.021922853,"about_ca_system_score_codex":0.00114949,"about_ca_system_score_gemma":0.00027928068,"threshold_uncertainty_score":0.043590486},"labels":[],"label_agreement":null},{"id":"W4405850184","doi":"10.3847/1538-4357/ad957b","title":"HETDEX-LOFAR Spectroscopic Redshift Catalog∗","year":2024,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Leibniz-Gemeinschaft; Science and Technology Facilities Council; Science Mission Directorate; DST-NRF Centre Of Excellence In Tree Health Biotechnology; Smithsonian Astrophysical Observatory; U.S. Air Force; Department of Mechanical Engineering, University of Texas at Austin; Gauss Centre for Supercomputing; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Leibniz-Institut für Astrophysik Potsdam; Eötvös Loránd Tudományegyetem; Ministerium für Innovation, Wissenschaft und Forschung des Landes Nordrhein-Westfalen; Ludwig-Maximilians-Universität München; Durham University; Istituto Nazionale di Astrofisica; Max-Planck-Gesellschaft; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Queen's University; Bundesministerium für Bildung und Forschung; National Science Foundation; Science Foundation Ireland; University of Hertfordshire; Space Telescope Science Institute; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; University of Tokyo; University of Texas at Austin; Centre National de la Recherche Scientifique; Pennsylvania State University; University of Oxford; Los Alamos National Laboratory; Johns Hopkins University; Missouri University of Science and Technology; National Central University; Gordon and Betty Moore Foundation; Queen's University Belfast; Université d'Orléans; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Physics; LOFAR; Redshift; Astrophysics; Astronomy; Quasar; Red shift; Galaxy; Radio telescope","score_opus":0.006666012885869948,"score_gpt":0.22346401459395418,"score_spread":0.21679800170808422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4405850184","genre_codex":"dataset","genre_gemma":"dataset","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"dataset","genre_consensus":"dataset","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.36204693,0.0006665046,0.027956199,0.00031725652,0.00013342872,0.0005216483,0.55594337,0.0068148994,0.045599684],"genre_scores_gemma":[0.16874363,0.0003027697,0.02101959,0.00023033856,0.00013890165,0.000516621,0.797265,0.00047472183,0.01130843],"study_design_codex":"observational","study_design_gemma":"not_applicable","domain_scores_codex":[0.998978,0.00007446691,0.00010490106,0.0002660219,0.00040119066,0.00017540266],"domain_scores_gemma":[0.9959422,0.0002827003,0.0011901616,0.0011893142,0.0010091778,0.00038650614],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013470921,0.00079309096,0.0004693202,0.00873014,0.0005411534,0.0013508474,0.00082830404,0.0002510333,0.018102596],"category_scores_gemma":[0.0025542837,0.00028130924,0.0003415079,0.004037462,0.00021809354,0.0010413161,0.0015307968,0.0003217416,0.01734738],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035070287,0.0003516604,0.58410645,0.00042997993,0.00021975407,0.00028060883,0.0005683619,0.00191322,0.015031445,0.009324419,0.21412109,0.17330238],"study_design_scores_gemma":[0.000111201516,0.00008114933,0.7008472,0.000082982275,0.00008804956,0.00034549116,0.00023193943,0.0024529842,0.008548836,0.0022648338,0.28487733,0.000067972884],"about_ca_topic_score_codex":0.00578032,"about_ca_topic_score_gemma":0.005487999,"teacher_disagreement_score":0.018102596,"about_ca_system_score_codex":0.00056847103,"about_ca_system_score_gemma":0.0007619939,"threshold_uncertainty_score":0.060559213},"labels":[],"label_agreement":null},{"id":"W4406042345","doi":"10.3847/1538-4357/ad900c","title":"Analysis of Polarized Dust Emission Using Data from the First Flight of SPIDER","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"British Antarctic Survey; Canadian Space Agency; Astrophysics Division; Norges Forskningsråd; Division of Antarctic Sciences; U.S. Department of Energy; European Commission; Flatiron Health; National Science Foundation; Compute Canada; Science Mission Directorate; Government of Ontario; National Aeronautics and Space Administration; University of Toronto; Research Corporation for Science Advancement; Vetenskapsrådet; Swedish National Space Agency","keywords":"Physics; Astrophysics; Planck; Cosmic microwave background; Spider; Black-body radiation; Polarization (electrochemistry); Computational physics; Anisotropy; Astronomy; Optics; Radiation","score_opus":0.020270746633259718,"score_gpt":0.29531531285542195,"score_spread":0.2750445662221622,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406042345","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975656,0.000037251808,0.00048611732,0.000013864565,0.0000030263461,0.0000048402403,0.0010717105,0.000040914085,0.00077662733],"genre_scores_gemma":[0.9957088,0.000042059473,0.0011806287,0.000013489414,0.0000085004085,0.000007471348,0.002859163,0.000016454445,0.00016330514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998671,0.000014277257,0.0000047513786,0.00004041646,0.00004010148,0.00003343371],"domain_scores_gemma":[0.9995746,0.000085418906,0.00009360502,0.00006825554,0.00007257821,0.00010546721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024988496,0.0002592749,0.00030058052,0.0012566671,0.00035227602,0.0004295611,0.00019764053,0.00022698862,0.00064159033],"category_scores_gemma":[0.0005027012,0.00015747364,0.00056005083,0.0007597763,0.00016294462,0.00022919486,0.00049867155,0.00024138854,0.00020591276],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00044929012,0.000102012884,0.89634913,0.00007969906,0.00029213598,0.0004645286,0.00060302374,0.003785736,0.075871006,0.00042015218,0.00094000326,0.020643404],"study_design_scores_gemma":[0.000008203591,0.00005437978,0.99007505,0.000005566444,0.000036067413,0.00018646482,0.00011456998,0.003187902,0.005168555,0.00008871614,0.001063262,0.0000111869595],"about_ca_topic_score_codex":0.004386897,"about_ca_topic_score_gemma":0.0069406005,"teacher_disagreement_score":0.004386897,"about_ca_system_score_codex":0.0002568761,"about_ca_system_score_gemma":0.00019058897,"threshold_uncertainty_score":0.0087227225},"labels":[],"label_agreement":null},{"id":"W4406089028","doi":"10.3847/1538-4357/ad972a","title":"PHANGS-ML: The Universal Relation between PAH Band and Optical Line Ratios across Nearby Star-forming Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency; National Institutes of Natural Sciences; Smithsonian Astrophysical Observatory; Agencia Nacional de Investigación y Desarrollo; National Astronomical Observatory of Japan; Deutsche Forschungsgemeinschaft; European Southern Observatory; Belgian Federal Science Policy Office; Space Telescope Science Institute; Agence Nationale de la Recherche; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Natural Sciences and Engineering Research Council of Canada; National Science Council; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Star (game theory); Line (geometry); Luminous infrared galaxy; Astronomy","score_opus":0.008642811063648247,"score_gpt":0.23686998648926239,"score_spread":0.22822717542561413,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406089028","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99465805,0.00011206043,0.001271693,0.000030383066,0.0000031775367,0.000006640079,0.0019688276,0.00022788256,0.0017213728],"genre_scores_gemma":[0.99853075,0.000016751888,0.00037705,0.000009726106,0.0000045106963,0.000003320097,0.00086641184,0.00001583226,0.00017569822],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997638,0.000036533907,0.000012752554,0.00012386685,0.000027266226,0.000035824647],"domain_scores_gemma":[0.9980678,0.00042594978,0.0005510174,0.00042381906,0.00023076178,0.0003006611],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036688097,0.000146563,0.000211724,0.00094951736,0.00021039581,0.0006070756,0.00025845206,0.0001700262,0.0037570002],"category_scores_gemma":[0.0016006487,0.00014483323,0.00014103242,0.0006859368,0.00031203876,0.0005272417,0.00046277163,0.00014725166,0.00064269593],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000069730064,0.00001359549,0.98082477,0.000021856871,0.000043254116,0.00005060899,0.00014027693,0.00029137966,0.0071949298,0.00020599837,0.0007294683,0.010414068],"study_design_scores_gemma":[0.0000025378467,0.000011144566,0.99801433,0.0000024218173,0.000006014084,0.000044288932,0.000061275074,0.00064718176,0.00059300585,0.000098941295,0.00051646563,0.0000024405697],"about_ca_topic_score_codex":0.0040531443,"about_ca_topic_score_gemma":0.0039952695,"teacher_disagreement_score":0.0040531443,"about_ca_system_score_codex":0.00016611132,"about_ca_system_score_gemma":0.00009712448,"threshold_uncertainty_score":0.012568414},"labels":[],"label_agreement":null},{"id":"W4406092706","doi":"10.3847/1538-4357/adb3a0","title":"Search for Continuous Gravitational Waves from Known Pulsars in the First Part of the Fourth LIGO-Virgo-KAGRA Observing Run","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Social Fund; Astrophysics Division; Astrophysics Science Division; National Research, Development and Innovation Office; Institute for Cosmic Ray Research, University of Tokyo; Institut National de Physique Nucléaire et de Physique des Particules; Great Southern Development Commission, Government of Western Australia; Agencia Estatal de Investigación; Fonds de recherche du Québec – Nature et technologies; Science and Engineering Research Board; Japan Society for the Promotion of Science; Smithsonian Astrophysical Observatory; Goddard Space Flight Center; National Science and Technology Council; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; National Astronomical Observatory of Japan; Conseil Régional, Île-de-France; Israel Science Foundation; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Observatoire de Paris, Université de Recherche Paris Sciences et Lettres; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Fonds Wetenschappelijk Onderzoek; Ministry of Education, India; Consejo Nacional de Investigaciones Científicas y Técnicas; Agencia Nacional de Investigación y Desarrollo; Istituto Nazionale di Fisica Nucleare; Smithsonian Institution; U.S. Department of Energy; Science and Technology Facilities Council; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Centre National d’Etudes Spatiales; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, Culture, Sports, Science and Technology; Council of Scientific and Industrial Research, India; Russian Science Foundation; Universidad Nacional de La Plata; European Commission; Leverhulme Trust; Scottish Funding Council; McGill Space Institute; Narodowa Agencja Wymiany Akademickiej; Centres de Recerca de Catalunya; Institut des Origines de Lyon; McGill University; Fonds De La Recherche Scientifique - FNRS; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; LIGO; Pulsar; Neutron star; Gravitational wave; Millisecond pulsar; Astrophysics; Amplitude; Binary pulsar; Astronomy; Crab Pulsar; General relativity; Chirp; Classical mechanics; Quantum mechanics","score_opus":0.017074104018052472,"score_gpt":0.3083397078999397,"score_spread":0.2912656038818872,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406092706","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99877363,0.000020017289,0.00042274257,0.0000139732665,0.0000016511822,0.0000066862995,0.00030198682,0.00003228244,0.0004270155],"genre_scores_gemma":[0.99595475,0.000019973111,0.0012729848,0.000012347986,0.000005955002,0.000017804618,0.0024273004,0.000015146507,0.00027384376],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99917895,0.0001284146,0.000036789785,0.00020872749,0.00024759313,0.00019951173],"domain_scores_gemma":[0.99738055,0.00065424526,0.00089203817,0.00043766518,0.00018817166,0.0004471637],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007074222,0.00043466303,0.0005396787,0.0018991153,0.0008016228,0.0008222387,0.00048244346,0.000372713,0.00085784803],"category_scores_gemma":[0.0018773084,0.0002434456,0.00054661714,0.0010570579,0.00041675204,0.00024611971,0.0013043346,0.00035470625,0.00026217732],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004177291,0.00010527435,0.9490415,0.000036078683,0.0002604842,0.00022452895,0.00033199653,0.0022063314,0.032137703,0.00028679264,0.0004930946,0.014458537],"study_design_scores_gemma":[0.000030437863,0.00019185728,0.9868569,0.000007588291,0.000138792,0.0001927517,0.00015910443,0.004575605,0.005801412,0.00019097558,0.0018378381,0.00001689835],"about_ca_topic_score_codex":0.0043936525,"about_ca_topic_score_gemma":0.007900034,"teacher_disagreement_score":0.0043936525,"about_ca_system_score_codex":0.0004903259,"about_ca_system_score_gemma":0.00055311224,"threshold_uncertainty_score":0.008736193},"labels":[],"label_agreement":null},{"id":"W4406188187","doi":"10.3847/1538-4357/ad9902","title":"Hot Spot Offset Variability from Magnetohydrodynamical Thermoresistive Instability in Hot Jupiters","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Hot Jupiter; Instability; Astronomy; Astrophysics; Offset (computer science); Plasma instability; Stellar wind; Hot spot (computer programming); Astrobiology; Mechanics; Stars; Exoplanet","score_opus":0.005176825090991256,"score_gpt":0.21221594879134387,"score_spread":0.2070391237003526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406188187","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977763,0.000042968037,0.0006944114,0.00006656143,0.0000063471307,0.000006408165,0.000112091766,0.00005336653,0.0012415773],"genre_scores_gemma":[0.999553,0.000012444139,0.00018530177,0.000011482328,0.0000035399087,0.000005372859,0.00009023002,0.000009961322,0.00012867394],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994814,0.000011805543,0.000002229249,0.000010909069,0.000007954382,0.000018891182],"domain_scores_gemma":[0.9998367,0.00005469495,0.000029799641,0.00001463846,0.00001656349,0.000047594083],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017973814,0.00037034863,0.0003244513,0.00023332107,0.00043063075,0.00060112367,0.00043762592,0.0006022591,0.0017720036],"category_scores_gemma":[0.0005915485,0.00022266906,0.00040245394,0.00016197475,0.00042290217,0.00035290848,0.00042455262,0.0004163883,0.00013406198],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003764572,0.00020701642,0.071857765,0.00006572154,0.00019520994,0.00079622533,0.0001853734,0.9016683,0.018092778,0.0015644395,0.0012873712,0.0037033178],"study_design_scores_gemma":[0.000094210984,0.00019400206,0.03924574,0.000011417008,0.000036646685,0.00009001171,0.00011416632,0.9571341,0.0016635866,0.0008533885,0.0005409973,0.000021648633],"about_ca_topic_score_codex":0.0073520946,"about_ca_topic_score_gemma":0.004527645,"teacher_disagreement_score":0.0073520946,"about_ca_system_score_codex":0.00044170974,"about_ca_system_score_gemma":0.00026439788,"threshold_uncertainty_score":0.014618576},"labels":[],"label_agreement":null},{"id":"W4406292376","doi":"10.3847/1538-4357/ad82df","title":"Determining the Nature of IC 10 X-2: A Comprehensive Study of the Optical/IR Emission from an Extragalactic BeHMXB","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta; Institute of Particle Physics","funders":"Agencia Estatal de Investigación; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Tamkeen; New York University Abu Dhabi","keywords":"Physics; Astrophysics; Astronomy; Emission spectrum; Infrared; Spectral line","score_opus":0.01142881489811901,"score_gpt":0.28255014555994024,"score_spread":0.2711213306618212,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406292376","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99677086,0.00055926724,0.000112354806,0.000015657306,0.0000015437593,0.000008234235,0.00036339794,0.000008252331,0.0021604549],"genre_scores_gemma":[0.9954543,0.000642791,0.00081412424,0.00008756613,0.000013157594,0.000007649809,0.002014193,0.000009020712,0.0009572016],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989927,0.00000779464,0.0000053387557,0.000027971106,0.00003132681,0.000028186481],"domain_scores_gemma":[0.9998611,0.00001154517,0.000049302846,0.000008853745,0.000021700234,0.000047471134],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016751213,0.00023387877,0.00015568726,0.0014552203,0.00027580533,0.0004891542,0.0001721569,0.00016518006,0.0007312162],"category_scores_gemma":[0.00011916111,0.000106550724,0.00014012477,0.0008265529,0.00014074841,0.0002114458,0.00040130998,0.0001793102,0.00022307198],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079434205,0.00008788432,0.90264785,0.00007979539,0.00006909773,0.00048553295,0.00036113724,0.00014591946,0.07787252,0.00008405629,0.00040754487,0.017679214],"study_design_scores_gemma":[7.433669e-7,0.000019316836,0.9984037,0.0000040012765,0.0000066973757,0.000101374026,0.00009052346,0.000038267513,0.0007290672,0.0000059002427,0.0005994976,9.1641283e-7],"about_ca_topic_score_codex":0.0057954337,"about_ca_topic_score_gemma":0.014907758,"teacher_disagreement_score":0.0057954337,"about_ca_system_score_codex":0.00021310507,"about_ca_system_score_gemma":0.00013818356,"threshold_uncertainty_score":0.011523366},"labels":[],"label_agreement":null},{"id":"W4406337410","doi":"10.3847/1538-4357/ad94ef","title":"The Effect of Galaxy Interactions on Starbursts in Milky Way-mass Galaxies in FIRE Simulations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"RES’EAU-WaterNET; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Interacting galaxy; Milky Way; Lenticular galaxy; Astronomy; Peculiar galaxy; Galaxy merger; Galaxy group; Elliptical galaxy","score_opus":0.005187935170193569,"score_gpt":0.24237979411268554,"score_spread":0.23719185894249198,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406337410","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989372,0.000036065285,0.00020337445,0.00004743093,0.000005253864,0.000005386479,0.0001880144,0.00004861091,0.0005286516],"genre_scores_gemma":[0.9984225,0.00003626254,0.0007273319,0.00004312876,0.000005296433,0.000013802353,0.0004933413,0.000033729688,0.0002246553],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999764,0.00007796876,0.000014990773,0.00004147644,0.00003683324,0.00006468986],"domain_scores_gemma":[0.9976913,0.0013386713,0.00026072297,0.0001764931,0.00017729001,0.0003555771],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012464396,0.0005169321,0.0006804908,0.0005929283,0.0005628193,0.0009258156,0.001446272,0.001103967,0.0011124914],"category_scores_gemma":[0.0049249004,0.00042552786,0.0010027225,0.0005087621,0.0006562399,0.0005750188,0.00071406004,0.0008711751,0.00014706924],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00071493717,0.00033544356,0.17629026,0.000056597004,0.00047881802,0.00021519414,0.00023102689,0.81334627,0.00290498,0.0015618644,0.0007909936,0.003073621],"study_design_scores_gemma":[0.0001705339,0.00026706114,0.037916426,0.000020354262,0.00010986434,0.000051169685,0.00014211539,0.95861053,0.0017611645,0.0004177581,0.00050837005,0.000024697974],"about_ca_topic_score_codex":0.02717839,"about_ca_topic_score_gemma":0.019129565,"teacher_disagreement_score":0.02717839,"about_ca_system_score_codex":0.00096718216,"about_ca_system_score_gemma":0.00069566956,"threshold_uncertainty_score":0.054040372},"labels":[],"label_agreement":null},{"id":"W4406337440","doi":"10.3847/1538-4357/ad9393","title":"Gravitational-wave Dark Siren Cosmology Systematics from Galaxy Weighting","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":16,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Cosmology; Astronomy; Astrophysics; Siren (mythology); Dark energy; Systematics; Galaxy; Dark matter; Galaxy formation and evolution","score_opus":0.009864257078793468,"score_gpt":0.2499224544833645,"score_spread":0.24005819740457104,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406337440","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7914872,0.00069290254,0.19864054,0.00029958677,0.00006198451,0.00007751183,0.0006780431,0.00070510275,0.0073570255],"genre_scores_gemma":[0.9896428,0.000059789814,0.00943244,0.00008316247,0.000016082193,0.00001544715,0.00041261918,0.00007097502,0.00026669892],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9962347,0.0020064097,0.00021339908,0.0009220392,0.00045793192,0.00016545242],"domain_scores_gemma":[0.9755525,0.010372832,0.0029565222,0.00913638,0.0015996966,0.0003819744],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.014109739,0.0005653118,0.00046365825,0.001361431,0.00050657004,0.0014528641,0.0008691099,0.0004619382,0.0013641021],"category_scores_gemma":[0.033173867,0.00046398677,0.0005719319,0.0008236011,0.0014558709,0.001441013,0.0019808344,0.0006235835,0.00024351456],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004879708,0.0000549339,0.81693447,0.0001916409,0.0011752355,0.00015950332,0.000769682,0.047282845,0.012671209,0.06309225,0.0018466985,0.05533369],"study_design_scores_gemma":[0.00007289717,0.00019478884,0.5693613,0.00013006509,0.00054528465,0.00035218833,0.00024216215,0.2942763,0.018243955,0.10866245,0.0077584875,0.0001600556],"about_ca_topic_score_codex":0.0021326016,"about_ca_topic_score_gemma":0.003443354,"teacher_disagreement_score":0.014109739,"about_ca_system_score_codex":0.00053649675,"about_ca_system_score_gemma":0.00034111564,"threshold_uncertainty_score":0.074620366},"labels":[],"label_agreement":null},{"id":"W4406404982","doi":"10.3847/1538-4357/ad9336","title":"PS1-11aop: Probing the Mass-loss History of a Luminous Interacting Supernova Prior to Its Final Eruption with Multiwavelength Observations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Research Council; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; Heising-Simons Foundation; National Science Foundation","keywords":"Physics; Supernova; Astrophysics; Astronomy","score_opus":0.029569466818537844,"score_gpt":0.25099487798602277,"score_spread":0.22142541116748493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406404982","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99915683,0.00005795456,0.000119532306,0.000008570272,0.0000016694947,0.000004053649,0.0002233179,0.000010021708,0.0004181145],"genre_scores_gemma":[0.9984804,0.00008204733,0.00039399206,0.000011156696,0.000005860128,0.0000052081105,0.00068869675,0.0000053887675,0.00032737968],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999316,0.0000046042087,0.0000033086233,0.000024169003,0.000016163594,0.000020082412],"domain_scores_gemma":[0.99972945,0.00002767715,0.00010005791,0.000020431413,0.0000349118,0.00008738358],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017501797,0.00022124272,0.00019560325,0.0007222642,0.00035257053,0.00044500394,0.00022554964,0.00021302055,0.0006085911],"category_scores_gemma":[0.0002580288,0.00016392407,0.00020579164,0.00038005406,0.000113433656,0.00024121093,0.00047363082,0.0003502078,0.00022864681],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001835278,0.000094092844,0.90785396,0.000033786895,0.00006815,0.0008932445,0.00020663158,0.00046505147,0.080077924,0.000095454896,0.0003024125,0.009725825],"study_design_scores_gemma":[0.0000013423222,0.00003292531,0.99759704,0.0000020931643,0.0000080538575,0.00024037051,0.000052966305,0.00031487847,0.0014127736,0.0000123422,0.000323341,0.0000018483371],"about_ca_topic_score_codex":0.0031877747,"about_ca_topic_score_gemma":0.0057704635,"teacher_disagreement_score":0.0031877747,"about_ca_system_score_codex":0.00019734056,"about_ca_system_score_gemma":0.0001178803,"threshold_uncertainty_score":0.0063384175},"labels":[],"label_agreement":null},{"id":"W4406687656","doi":"10.3847/1538-4357/ad95f6","title":"Detecting Stellar Flares in Photometric Data Using Hidden Markov Models","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Astronomy","score_opus":0.028366601825855264,"score_gpt":0.28262549075018795,"score_spread":0.2542588889243327,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406687656","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.33354747,0.00019821283,0.66245884,0.0002820503,0.000027420927,0.00003760721,0.0007816764,0.0016700645,0.0009967665],"genre_scores_gemma":[0.94609636,0.00006307722,0.052629996,0.00004188135,0.000014341066,0.000021562742,0.0006192954,0.000044835262,0.0004687253],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99975294,0.00006180492,0.000014991879,0.000064130174,0.00007331513,0.000032757394],"domain_scores_gemma":[0.9980141,0.0013942788,0.00022025881,0.00016225061,0.00014860356,0.000060519556],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00094337255,0.00028689293,0.00039162548,0.0008597022,0.0002784254,0.0006221816,0.0005263805,0.00054847065,0.00067064894],"category_scores_gemma":[0.003504366,0.00024974442,0.00044418176,0.00056597625,0.00026974804,0.0006074989,0.00051262055,0.0006857775,0.00025446093],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003956233,0.00017838382,0.07211423,0.00008117156,0.00014898684,0.00025288542,0.00023832177,0.7713513,0.016076963,0.0048890803,0.0014912516,0.1327818],"study_design_scores_gemma":[0.0000023047758,0.000007982007,0.0030775815,0.000003294249,0.000004736522,0.000012041613,0.000008837459,0.9944126,0.0012529474,0.0010822534,0.00012866787,0.0000066724865],"about_ca_topic_score_codex":0.009329833,"about_ca_topic_score_gemma":0.008898111,"teacher_disagreement_score":0.009329833,"about_ca_system_score_codex":0.0005645329,"about_ca_system_score_gemma":0.0004413219,"threshold_uncertainty_score":0.018551052},"labels":[],"label_agreement":null},{"id":"W4406696544","doi":"10.3847/1538-4357/ad9aa1","title":"On the Formation of Planets in the Milky Way’s Thick Disk","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Milky Way; Planet; Astronomy; Astrobiology; Astrophysics; Exoplanet; Stars","score_opus":0.010920903705271072,"score_gpt":0.2274770795568453,"score_spread":0.21655617585157422,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406696544","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996001,0.00010862461,0.000012482142,0.000012741677,4.2251799e-7,3.8841634e-7,0.000021073129,7.288824e-7,0.00024332023],"genre_scores_gemma":[0.9997811,0.00004173422,0.000015781943,0.000003751612,9.308829e-7,3.8689274e-7,0.00005726374,6.553627e-7,0.00009847154],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999187,0.000015372829,0.0000046252035,0.00002230141,0.00001317089,0.000025906482],"domain_scores_gemma":[0.9991768,0.00015831909,0.00038467007,0.000053489923,0.000060766728,0.00016584547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023598659,0.00013371014,0.00013232797,0.00071378885,0.0003663146,0.00077729375,0.00024565108,0.00027905896,0.0008903116],"category_scores_gemma":[0.001363193,0.00010542736,0.00015187495,0.0003170197,0.0004406886,0.00041501757,0.0007477319,0.00012847691,0.0001549707],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009896377,0.000019201183,0.99109906,0.000019903353,0.00004552188,0.00038429865,0.0003790707,0.00067309104,0.003757533,0.0005160046,0.00008673718,0.0029207682],"study_design_scores_gemma":[0.0000029956109,0.00002843417,0.9977476,0.0000066077923,0.00001530711,0.00015834688,0.00036278123,0.0006338008,0.0004158978,0.00016602605,0.0004597269,0.0000024105188],"about_ca_topic_score_codex":0.005250863,"about_ca_topic_score_gemma":0.0057661454,"teacher_disagreement_score":0.005250863,"about_ca_system_score_codex":0.00048115,"about_ca_system_score_gemma":0.00013805371,"threshold_uncertainty_score":0.010440588},"labels":[],"label_agreement":null},{"id":"W4406732168","doi":"10.3847/1538-4357/ad9b17","title":"What Does the LMC Look Like? It Depends on [M/H] and Age","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Large Magellanic Cloud; Astronomy; Stars","score_opus":0.007966969287005424,"score_gpt":0.23317155639699347,"score_spread":0.22520458710998803,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406732168","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.60542417,0.0116957305,0.008098155,0.05556644,0.001717773,0.000077675584,0.023720603,0.0021784771,0.29152092],"genre_scores_gemma":[0.96756035,0.0022223766,0.0037091451,0.0054462906,0.0010259872,0.000043272335,0.0034882578,0.00077082415,0.015733639],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958783,0.0001027749,0.000014806877,0.00012446678,0.00010020024,0.00006995944],"domain_scores_gemma":[0.99828476,0.00025537008,0.00024869098,0.00018499413,0.0006183756,0.00040781545],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00059389183,0.00026697197,0.00032203775,0.0014047687,0.0010564685,0.0040898407,0.00048763535,0.0007414275,0.0110114105],"category_scores_gemma":[0.0034254766,0.0001485277,0.00024612114,0.0017973996,0.0011597316,0.0025250895,0.00068415795,0.0008714907,0.0049395105],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032837235,0.00004484251,0.5207278,0.00043589354,0.00031561375,0.0006457399,0.0026037989,0.0021038349,0.006394124,0.020013468,0.27773517,0.16865136],"study_design_scores_gemma":[0.000013673641,0.000036751302,0.8642907,0.00025962156,0.00006709874,0.0003272712,0.0030738697,0.0016378509,0.0013807762,0.011734605,0.117062815,0.00011503489],"about_ca_topic_score_codex":0.028157325,"about_ca_topic_score_gemma":0.030971015,"teacher_disagreement_score":0.028157325,"about_ca_system_score_codex":0.0015744503,"about_ca_system_score_gemma":0.00047271836,"threshold_uncertainty_score":0.05598688},"labels":[],"label_agreement":null},{"id":"W4406766248","doi":"10.3847/1538-4357/ad8eba","title":"Discovery and Spectroscopic Confirmation of Aquarius III: A Low-mass Milky Way Satellite Galaxy","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Science and Technology Facilities Council; Astrophysics Division; Natural Sciences and Engineering Research Council of Canada; Kavli Institute for Cosmological Physics, University of Chicago; Office of Science; University of Illinois at Urbana-Champaign; Centro de Investigaciones Energéticas, Medioambientales y Tecnológicas; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Chinese Academy of Sciences; High Energy Physics; Deutsche Forschungsgemeinschaft; Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Nuclear Safety and Security Commission; Center for Cosmology and Astroparticle Physics, Ohio State University; University of Sussex; University of Toronto; Yale University; University of Portsmouth; NASA Exoplanet Science Institute; Jet Propulsion Laboratory; University of California, Santa Cruz; Ohio State University; University College London; National Aeronautics and Space Administration; California Institute of Technology; U.S. Department of Energy; W. M. Keck Foundation; European Space Agency; Fermilab; Laboratory Directed Research and Development; National Science Foundation; Institut de Física d'Altes Energies; Eidgenössische Technische Hochschule Zürich; National Centre for Supercomputing Applications","keywords":"Algorithm; Computer science","score_opus":0.004403848888926828,"score_gpt":0.2104071237775372,"score_spread":0.20600327488861037,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406766248","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9922093,0.00019161552,0.00069627055,0.00020469859,0.000024829274,0.000015689315,0.0005320157,0.00011775968,0.006007714],"genre_scores_gemma":[0.99610007,0.000044639433,0.0010632616,0.00016015813,0.000022585498,0.0000071646377,0.00091311947,0.00002315552,0.0016658474],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99988174,0.000007697328,0.0000060735556,0.000038480106,0.000035423276,0.000030641066],"domain_scores_gemma":[0.9996332,0.000021685937,0.000074104144,0.000049519407,0.000041641746,0.00017988229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018787372,0.00023761534,0.00015848079,0.0005650828,0.00055302685,0.0006420592,0.00041115473,0.0004229308,0.0025577752],"category_scores_gemma":[0.00032947387,0.00013931104,0.00022683477,0.00029288518,0.0004283254,0.00022997678,0.0009969111,0.00035361215,0.0009471831],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00041474047,0.00012187163,0.7217152,0.000099522615,0.000124622,0.003812093,0.0011708253,0.00035363573,0.23053557,0.0032310341,0.0058045997,0.0326162],"study_design_scores_gemma":[0.000050545237,0.0004573185,0.91540724,0.0000383108,0.00006369798,0.0057129553,0.0008907393,0.001226242,0.028966479,0.0014580621,0.04569133,0.000037017264],"about_ca_topic_score_codex":0.0028615205,"about_ca_topic_score_gemma":0.0031017708,"teacher_disagreement_score":0.0028615205,"about_ca_system_score_codex":0.00037378955,"about_ca_system_score_gemma":0.00020484238,"threshold_uncertainty_score":0.008556664},"labels":[],"label_agreement":null},{"id":"W4406772821","doi":"10.3847/1538-4357/ada1d3","title":"Cosmic Reionization on Computers: The Evolution of the Ionizing Background and Mean Free Path","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Reionization; Physics; Ionizing radiation; Mean free path; Astronomy; COSMIC cancer database; Astrophysics; Cosmic ray; Background radiation; Intergalactic medium; Nuclear physics; Radiation; Galaxy; Redshift","score_opus":0.008476401119310266,"score_gpt":0.23436763556760648,"score_spread":0.2258912344482962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406772821","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99740964,0.000040416024,0.0011197254,0.0000596002,0.0000053244476,0.000006318501,0.00014859784,0.00011515936,0.0010952358],"genre_scores_gemma":[0.9980071,0.000027213619,0.001470533,0.000017720116,0.0000021727533,0.000009165466,0.00024203636,0.000034127635,0.00018992001],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997633,0.00006958728,0.000008918299,0.000049297785,0.00004360691,0.00006525685],"domain_scores_gemma":[0.9974668,0.0014500914,0.000336666,0.0002589448,0.00023605405,0.00025152424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00062526384,0.0004479474,0.00033504525,0.0004942891,0.00032648994,0.00073999626,0.0006853293,0.000458745,0.0009179434],"category_scores_gemma":[0.0033689796,0.00022145588,0.00032868987,0.000543792,0.00061885786,0.00058578583,0.00045145952,0.00070323487,0.000081486214],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022076156,0.00012633772,0.05398823,0.00002774578,0.00008923223,0.00011299757,0.00011245619,0.9333774,0.0045603085,0.0026984557,0.00067765836,0.00400851],"study_design_scores_gemma":[0.000026867863,0.00008053908,0.0113031175,0.000006222091,0.000017546541,0.00002262408,0.000050237297,0.98494476,0.002449307,0.0007298061,0.00035755007,0.0000115376315],"about_ca_topic_score_codex":0.014210732,"about_ca_topic_score_gemma":0.007135772,"teacher_disagreement_score":0.014210732,"about_ca_system_score_codex":0.00086775987,"about_ca_system_score_gemma":0.0005042328,"threshold_uncertainty_score":0.028256059},"labels":[],"label_agreement":null},{"id":"W4406803298","doi":"10.3847/1538-4357/ad9b0c","title":"A Pride of Satellites in the Constellation Leo? Discovery of the Leo VI Milky Way Satellite Ultra-faint Dwarf Galaxy with DELVE Early Data Release 3","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":17,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Fermilab; Laboratory Directed Research and Development; Natural Sciences and Engineering Research Council of Canada; University of Illinois at Urbana-Champaign; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; Conselho Nacional de Desenvolvimento Científico e Tecnológico; Science and Technology Facilities Council; University of Toronto; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia e Inovação; Deutsche Forschungsgemeinschaft; Ohio State University; National Science Foundation; Yale University; Argonne National Laboratory; U.S. Department of Energy","keywords":"Algorithm; Computer science","score_opus":0.012914420935737282,"score_gpt":0.231067705498393,"score_spread":0.21815328456265573,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406803298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9714036,0.0012117653,0.0012227972,0.00215985,0.00010407791,0.000013976614,0.0010189619,0.00013448455,0.022730472],"genre_scores_gemma":[0.9906679,0.00032596258,0.0017437132,0.00065755326,0.000077655684,0.000007394733,0.0016476595,0.000056286026,0.0048158946],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968946,0.000026865375,0.000010999933,0.0000922599,0.000107520755,0.00007293697],"domain_scores_gemma":[0.999102,0.000115334406,0.00021544386,0.0001773001,0.00014295023,0.00024697205],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00054179004,0.0001500274,0.00019028937,0.000712972,0.00057441456,0.0015521294,0.00029067227,0.00038313048,0.0021357303],"category_scores_gemma":[0.0011376006,0.00016535925,0.00015929785,0.00053851533,0.00076632673,0.0009030935,0.0017138411,0.000640022,0.00058318896],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006437358,0.000067014924,0.8501574,0.00015418601,0.00014861363,0.0028321552,0.005251787,0.00051960617,0.039669238,0.00991892,0.017101254,0.07353626],"study_design_scores_gemma":[0.00004295316,0.0001883679,0.72097164,0.00016123703,0.00005435192,0.0025346573,0.0035700875,0.0009007474,0.007119134,0.002744858,0.2616544,0.0000576803],"about_ca_topic_score_codex":0.0055417335,"about_ca_topic_score_gemma":0.010158648,"teacher_disagreement_score":0.0055417335,"about_ca_system_score_codex":0.0007116517,"about_ca_system_score_gemma":0.0002334804,"threshold_uncertainty_score":0.0110189915},"labels":[],"label_agreement":null},{"id":"W4406806306","doi":"10.3847/1538-4357/ada144","title":"A Second Candidate Magnetic Helium Core White Dwarf and 3 Other Variable White Dwarfs in the Globular Cluster NGC 6397","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Globular cluster; White dwarf; Astrophysics; Open cluster; Blue dwarf; Astronomy; Massive compact halo object; Variable star; Horizontal branch; Blue straggler; Helium; Stars","score_opus":0.007071822168550007,"score_gpt":0.2196812364590579,"score_spread":0.2126094142905079,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406806306","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995492,0.00001773929,0.00006457569,0.000008212799,0.0000012617204,0.000001161446,0.00007369819,0.0000046839855,0.0002794032],"genre_scores_gemma":[0.99939585,0.000012958369,0.00011869826,0.000007803312,0.0000024335448,0.0000019160461,0.00026648035,0.0000021225248,0.00019176312],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999881,0.000006586117,0.000011168011,0.000032233038,0.000041669904,0.000027273636],"domain_scores_gemma":[0.9995277,0.000079897094,0.00013625501,0.00006670288,0.000046829577,0.00014260363],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019175795,0.00015946486,0.00029104468,0.0011127478,0.0007190535,0.00062568946,0.00035817054,0.00032223616,0.0009811714],"category_scores_gemma":[0.0003976615,0.00009869653,0.00018648324,0.0009258889,0.00036671996,0.00014418409,0.0004614213,0.0002150597,0.00025542956],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016020032,0.000052282747,0.9602781,0.000018452673,0.000040560415,0.0027087717,0.0006107418,0.00016271163,0.027922053,0.00023785517,0.00024328523,0.0075650867],"study_design_scores_gemma":[0.000007718882,0.000038343074,0.99422234,0.000005384703,0.000013902829,0.0014383562,0.00039652016,0.0003714788,0.0026786025,0.00012203126,0.0006986173,0.000006623045],"about_ca_topic_score_codex":0.0062457086,"about_ca_topic_score_gemma":0.0116805015,"teacher_disagreement_score":0.0062457086,"about_ca_system_score_codex":0.0003648277,"about_ca_system_score_gemma":0.00021817672,"threshold_uncertainty_score":0.012418687},"labels":[],"label_agreement":null},{"id":"W4406816035","doi":"10.3847/1538-4357/ad9338","title":"What Rogue Hydrogen Clouds Tell Us about Galactic Magnetic Fields","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Research Council Canada; Natural Sciences and Engineering Research Council of Canada; Centre National de la Recherche Scientifique; University of Toronto","keywords":"Physics; Astronomy; Astrophysics; Magnetic field; Molecular cloud; Hydrogen; Astrobiology; Stars","score_opus":0.005386905783158837,"score_gpt":0.22173578711895015,"score_spread":0.2163488813357913,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406816035","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94904804,0.01811136,0.0010575915,0.009662165,0.00041139062,0.0000070156448,0.0011538374,0.000056893878,0.020491723],"genre_scores_gemma":[0.9950054,0.0026555434,0.00010764853,0.0007328544,0.0005954208,0.00000137712,0.00021211721,0.000015669963,0.00067399465],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998078,0.000054224853,0.000008659857,0.00004760315,0.00004211188,0.00003964191],"domain_scores_gemma":[0.99832493,0.00056793663,0.0005114755,0.00020731647,0.00016068143,0.0002276114],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006243617,0.00017490002,0.00031979298,0.0014154399,0.0005284106,0.0026129559,0.00037439747,0.0009811808,0.0025082796],"category_scores_gemma":[0.004675729,0.00016822907,0.00015124053,0.0011217801,0.0018568989,0.00430202,0.0005921284,0.0009999941,0.0007892393],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006664563,0.000053084234,0.8832119,0.00024094153,0.00041421544,0.0010422565,0.010310525,0.0005785644,0.00819437,0.00930534,0.010038761,0.075943455],"study_design_scores_gemma":[0.000032744123,0.00013601838,0.90354794,0.00026984882,0.000084755404,0.0018087947,0.02243248,0.0007937822,0.0018677175,0.035729133,0.033219878,0.000076807526],"about_ca_topic_score_codex":0.0025975755,"about_ca_topic_score_gemma":0.0035710386,"teacher_disagreement_score":0.0026129559,"about_ca_system_score_codex":0.00045564954,"about_ca_system_score_gemma":0.00011033013,"threshold_uncertainty_score":0.008391023},"labels":[],"label_agreement":null},{"id":"W4406816217","doi":"10.3847/1538-4357/ad969a","title":"Data-driven Dynamics with Orbital Torus Imaging: A Flexible Model of the Vertical Phase Space of the Galaxy","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; Office of Science; Alfred P. Sloan Foundation; U.S. Department of Energy","keywords":"Physics; Torus; Orbital mechanics; Phase space; Astronomy; Space (punctuation); Astrophysics; Galaxy; Dynamics (music); Stellar dynamics; Satellite; Geometry","score_opus":0.014662614123240096,"score_gpt":0.2568813150477463,"score_spread":0.2422187009245062,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406816217","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07415782,0.000116533294,0.9182885,0.0006789741,0.00004322668,0.000050920895,0.0008039583,0.0015777318,0.0042822766],"genre_scores_gemma":[0.7953371,0.00022631341,0.19885722,0.0001683974,0.00008562898,0.00022147478,0.0011792567,0.0006408946,0.003283709],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99964154,0.000104873565,0.00001960512,0.00009409982,0.000083011604,0.000056766097],"domain_scores_gemma":[0.99847895,0.0006483351,0.00019544605,0.00036469617,0.00015533474,0.00015730581],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001502611,0.00044371412,0.0005162125,0.0007030158,0.00052923453,0.0018175503,0.002171904,0.0009770632,0.0023707512],"category_scores_gemma":[0.006037753,0.00049256324,0.0012014495,0.0006566725,0.0013878655,0.0024359168,0.0017042388,0.00084437686,0.00048170917],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012043629,0.00002946859,0.0071788756,0.00005002208,0.00004181403,0.00015171728,0.00027084578,0.82490814,0.0020743632,0.15024318,0.0016085255,0.013322573],"study_design_scores_gemma":[0.000007448632,0.000008447798,0.00019912588,0.0000054945926,0.0000026532637,0.00002191794,0.000009775284,0.9811426,0.00017509848,0.017539479,0.0008824831,0.000005458961],"about_ca_topic_score_codex":0.010724731,"about_ca_topic_score_gemma":0.00600913,"teacher_disagreement_score":0.010724731,"about_ca_system_score_codex":0.0014126208,"about_ca_system_score_gemma":0.0011541233,"threshold_uncertainty_score":0.021324575},"labels":[],"label_agreement":null},{"id":"W4406933253","doi":"10.3847/1538-4357/ad9f2c","title":"Vortex-induced Rings and Gaps within Protoplanetary Disks","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Protoplanetary disk; Vortex; Astrophysics; Astronomy; Accretion disc; Astrobiology; Planet; Mechanics","score_opus":0.008598211308336252,"score_gpt":0.2414839147479894,"score_spread":0.23288570343965315,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4406933253","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985738,0.000042011197,0.0004864875,0.000038677732,0.0000068995732,0.000005274787,0.000033075372,0.000025043506,0.00078860554],"genre_scores_gemma":[0.9996195,0.000014955893,0.00020270524,0.0000061924184,0.0000020652708,0.0000026495343,0.000021111757,0.000004598787,0.00012633503],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999635,0.0000052031187,0.0000016897208,0.000006945617,0.0000064869128,0.000016184335],"domain_scores_gemma":[0.99980766,0.00003670031,0.000060383718,0.000018575074,0.00001829217,0.000058382804],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012580593,0.00015608412,0.00019039826,0.00019484303,0.00038574886,0.0005865756,0.0002323689,0.00031400268,0.0011558243],"category_scores_gemma":[0.00034430885,0.00017565761,0.00020221445,0.00009347819,0.0005050833,0.00036288679,0.000360584,0.00021126927,0.000095420095],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00072286977,0.0005530552,0.09343086,0.00015509271,0.00018106254,0.0014296527,0.00052145886,0.79196095,0.08793579,0.014212663,0.0019285757,0.006967906],"study_design_scores_gemma":[0.00024687473,0.00029839898,0.057780974,0.000017725719,0.000035750538,0.00015534213,0.00028608541,0.92739403,0.008761279,0.0038112653,0.001184103,0.000028257384],"about_ca_topic_score_codex":0.0019830575,"about_ca_topic_score_gemma":0.0009532334,"teacher_disagreement_score":0.0019830575,"about_ca_system_score_codex":0.00042688978,"about_ca_system_score_gemma":0.00026738006,"threshold_uncertainty_score":0.003943026},"labels":[],"label_agreement":null},{"id":"W4407153215","doi":"10.3847/1538-4357/ada1d8","title":"Associations between Scattering Screens and Interstellar Medium Filaments","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; University of Toronto; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Interstellar medium; Scattering; Astronomy; Interstellar cloud; Astrophysics; Astrobiology; Galaxy; Optics","score_opus":0.012962008780348318,"score_gpt":0.26088007508195976,"score_spread":0.24791806630161145,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407153215","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987072,0.00013837537,0.00045228342,0.00001148542,0.0000030832298,0.0000043021473,0.00009174234,0.000013930878,0.0005775827],"genre_scores_gemma":[0.9996339,0.000025521538,0.00017073435,0.000004520165,0.0000036254035,0.0000015046159,0.00008123547,0.0000017452718,0.00007736514],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992398,0.00014327295,0.000080041464,0.00018450303,0.0002222312,0.0001301478],"domain_scores_gemma":[0.9906441,0.0031467064,0.0045372117,0.0006425093,0.00049915427,0.0005303564],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006048993,0.00018603622,0.00026518226,0.0013734846,0.00032715764,0.0010900674,0.00019899083,0.00032128458,0.0016953528],"category_scores_gemma":[0.004058761,0.0001945835,0.00025022874,0.0010278852,0.000595053,0.00037456417,0.0005439879,0.00026829986,0.0001570641],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012616484,0.000013633485,0.9896931,0.000013545073,0.000066286295,0.00014894504,0.00005219893,0.00015010493,0.0071984082,0.00009805864,0.000042859527,0.0023967319],"study_design_scores_gemma":[0.0000030335743,0.000046761703,0.996407,0.0000045794727,0.000034828714,0.00046201993,0.00011293589,0.0004318358,0.0021225978,0.00015819687,0.00021076316,0.0000054084676],"about_ca_topic_score_codex":0.0014713879,"about_ca_topic_score_gemma":0.0017485331,"teacher_disagreement_score":0.0016953528,"about_ca_system_score_codex":0.0002243629,"about_ca_system_score_gemma":0.00017211933,"threshold_uncertainty_score":0.0056715608},"labels":[],"label_agreement":null},{"id":"W4407156703","doi":"10.3847/1538-4357/ada690","title":"GD-1 Stellar Stream and Cocoon in the DESI Early Data Release","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":14,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; High Energy Physics; Division of Astronomical Sciences; Science and Technology Facilities Council; Jet Propulsion Laboratory; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministerio de Ciencia e Innovación; Chinese Academy of Sciences; California Institute of Technology; U.S. Department of Energy; Gordon and Betty Moore Foundation; Nuclear Safety and Security Commission; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Alfred P. Sloan Foundation; National Science Foundation; European Space Agency; National Aeronautics and Space Administration; Consejo Nacional de Ciencia y Tecnología","keywords":"Physics; Astrophysics; Analytical Chemistry (journal); Chromatography; Chemistry","score_opus":0.017899143935724122,"score_gpt":0.25102091038355234,"score_spread":0.23312176644782823,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407156703","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98133564,0.00022456117,0.0011851115,0.00016953029,0.000047490317,0.000031779735,0.0074752173,0.0005341123,0.008996618],"genre_scores_gemma":[0.97478354,0.00013773287,0.0026109703,0.00013801319,0.00004849827,0.000023654908,0.018518817,0.00020943611,0.0035293407],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99983907,0.000008965553,0.000009051378,0.000048568007,0.00006046047,0.000033918353],"domain_scores_gemma":[0.9995956,0.000036861893,0.00010536447,0.00007479758,0.00009319431,0.00009425455],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00024702647,0.00023763801,0.00023381635,0.0010557923,0.00044891366,0.0006047601,0.00024271186,0.00019472066,0.001716207],"category_scores_gemma":[0.000722236,0.00012637126,0.00013566327,0.0009814926,0.00020265183,0.0003154799,0.0007048287,0.0002389977,0.0011224813],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000550895,0.00006886513,0.91550916,0.00006942317,0.000038298556,0.00064095366,0.00063725526,0.0007609034,0.021867119,0.0009411597,0.012257262,0.046658754],"study_design_scores_gemma":[0.00003703434,0.000057427016,0.94596505,0.00001809912,0.00002647836,0.00039335783,0.00019463843,0.0036654912,0.0070951595,0.00034615767,0.042185362,0.000015732106],"about_ca_topic_score_codex":0.0067879325,"about_ca_topic_score_gemma":0.013900301,"teacher_disagreement_score":0.0067879325,"about_ca_system_score_codex":0.00062873395,"about_ca_system_score_gemma":0.00022397068,"threshold_uncertainty_score":0.013496816},"labels":[],"label_agreement":null},{"id":"W4407217255","doi":"10.3847/1538-4357/ad9b92","title":"Tackling the Problem of Distributional Shifts: Correcting Misspecified, High-dimensional Data-driven Priors for Inverse Problems","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Statistical and numerical algorithms","field":"Mathematics","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canada Research Chairs; Compute Canada; Schmidt Futures","keywords":"Physics; Prior probability; Inverse problem; Inverse; Statistical physics; Applied mathematics; Bayesian probability; Astrophysics; Econometrics; Statistics; Mathematical analysis; Geometry; Economics","score_opus":0.044183959764820015,"score_gpt":0.3092029314578816,"score_spread":0.26501897169306154,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407217255","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.01553028,0.00017476195,0.98313844,0.00037540717,0.000026900403,0.00001957266,0.000036940186,0.00028548605,0.00041231394],"genre_scores_gemma":[0.462693,0.00046596013,0.5327122,0.0007381048,0.00011859856,0.00013669943,0.00039007538,0.0005278834,0.002217297],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9981122,0.0007366593,0.00010479494,0.00037500428,0.00054315827,0.00012818188],"domain_scores_gemma":[0.98730576,0.008114472,0.0013317,0.0016489858,0.0012448148,0.00035410476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0070649055,0.0014360189,0.0012841797,0.0010143438,0.0007261612,0.0016526859,0.0026305278,0.0028314644,0.0015262964],"category_scores_gemma":[0.032081917,0.0013955635,0.00097645726,0.00079419627,0.0029106669,0.002603891,0.0040860823,0.004410907,0.00060675945],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000110641944,0.000059368653,0.0028908267,0.00017842889,0.00011418371,0.00020834287,0.00028852478,0.909748,0.00883133,0.028076803,0.0014601331,0.048033398],"study_design_scores_gemma":[0.000012501975,0.000023483404,0.00038951339,0.000024967172,0.000010913332,0.00007319416,0.000026916,0.9781563,0.0028404004,0.017522452,0.00089941715,0.00001975663],"about_ca_topic_score_codex":0.008623053,"about_ca_topic_score_gemma":0.009056942,"teacher_disagreement_score":0.008623053,"about_ca_system_score_codex":0.0012234377,"about_ca_system_score_gemma":0.0023590175,"threshold_uncertainty_score":0.03736323},"labels":[],"label_agreement":null},{"id":"W4407262104","doi":"10.3847/1538-4357/ada9ea","title":"Shaping Outflows and Jets by Ambient Pressure: A Unified Framework","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Outflow; Astrophysics; Supersonic speed; Young stellar object; Astrophysical jet; Jet (fluid); Active galactic nucleus; Astronomy; Stars; Star formation; Mechanics; Galaxy","score_opus":0.011166713525426803,"score_gpt":0.2555038404259033,"score_spread":0.2443371269004765,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407262104","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.2207196,0.0024366786,0.7130306,0.0024039627,0.00029560743,0.00008360708,0.00043297044,0.0007452457,0.05985167],"genre_scores_gemma":[0.97045386,0.0011199908,0.022941386,0.00020812622,0.000384912,0.000074503405,0.00009793587,0.00012527501,0.004594075],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99978393,0.000066405446,0.000009630963,0.000049356942,0.000040107472,0.000050447194],"domain_scores_gemma":[0.99960953,0.000083337014,0.00007887872,0.00007041009,0.000062510895,0.000095304546],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004543917,0.00086698163,0.0010566561,0.0007082158,0.000949826,0.0033285678,0.00147099,0.0017127605,0.0020551132],"category_scores_gemma":[0.0008221909,0.0005488534,0.001175709,0.00034948907,0.0028856557,0.0029852872,0.0021221552,0.0010687455,0.00036995235],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000034591078,0.00008380215,0.0019238794,0.00006688953,0.00003704122,0.00032448085,0.00015202202,0.25734234,0.006932412,0.7263188,0.0010380876,0.0057456205],"study_design_scores_gemma":[0.000034126686,0.000051022125,0.0017231392,0.000017508406,0.000018575567,0.0001012494,0.00006152507,0.767546,0.00033083896,0.22791764,0.0021574046,0.000040917042],"about_ca_topic_score_codex":0.0022766655,"about_ca_topic_score_gemma":0.0013074391,"teacher_disagreement_score":0.0033285678,"about_ca_system_score_codex":0.0008422008,"about_ca_system_score_gemma":0.0006651319,"threshold_uncertainty_score":0.006875038},"labels":[],"label_agreement":null},{"id":"W4407386520","doi":"10.3847/1538-4357/ada8a2","title":"Improved SED-fitting Assumptions Result in Inside-out Quenching at z ~ 0.5 and Quenching at All Radii Simultaneously at z ~ 1","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Maryland Advanced Research Computing Center; Maryland Space Grant Consortium; Johns Hopkins University; National Aeronautics and Space Administration; Canadian Space Agency; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Quenching (fluorescence); sed; Astrophysics; Optics; Medicine","score_opus":0.00856640844918459,"score_gpt":0.2377207227951248,"score_spread":0.2291543143459402,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407386520","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.95893574,0.00014708003,0.037178803,0.0001935646,0.000010216497,0.00002097513,0.00053906057,0.0014514411,0.0015231628],"genre_scores_gemma":[0.99407333,0.000020361053,0.0050539295,0.00007716677,0.00000438238,0.000007382841,0.00042870815,0.00012276287,0.00021197065],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99928695,0.0001316844,0.000051367206,0.00025232302,0.0001495914,0.00012804887],"domain_scores_gemma":[0.9952289,0.0015309851,0.00119628,0.0012028455,0.0005561914,0.00028489385],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.002807653,0.0004745314,0.00050437247,0.0005573717,0.0004928852,0.0012314299,0.00090475706,0.0007684196,0.0016337795],"category_scores_gemma":[0.008611296,0.00032054662,0.0008540827,0.0005514848,0.00044588457,0.0011673677,0.00066128647,0.00080070936,0.00060552836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040645112,0.00013290218,0.8021188,0.00009475039,0.00046089504,0.00025200206,0.0007996425,0.08770605,0.059549693,0.0030591749,0.0016858347,0.04373375],"study_design_scores_gemma":[0.00003708476,0.00013548428,0.795696,0.000027439466,0.00014167615,0.00020931348,0.00018873326,0.1793297,0.019599142,0.0019346237,0.0026577534,0.000043007916],"about_ca_topic_score_codex":0.007392023,"about_ca_topic_score_gemma":0.0070222877,"teacher_disagreement_score":0.007392023,"about_ca_system_score_codex":0.00091613905,"about_ca_system_score_gemma":0.00033801293,"threshold_uncertainty_score":0.014848411},"labels":[],"label_agreement":null},{"id":"W4407417528","doi":"10.3847/1538-4357/ada7ed","title":"Hubble Space Telescope Observations within the Sphere of Influence of the Powerful Supermassive Black Hole in PKS 0745-191","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; University of Waterloo; Centre for Research in Astrophysics of Québec; Université de Montréal","funders":"Fonds de recherche du Québec – Nature et technologies; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs","keywords":"Physics; Supermassive black hole; Astrophysics; Hubble space telescope; Astronomy; Black hole (networking); Quasar; Galaxy","score_opus":0.006941444693360357,"score_gpt":0.2151694018549236,"score_spread":0.20822795716156323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407417528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99854326,0.00006535478,0.00017470443,0.000014338466,0.0000029631312,0.000003365368,0.00020002894,0.00002902666,0.00096689817],"genre_scores_gemma":[0.99935895,0.00003367011,0.00021226026,0.000011931804,0.0000068268114,0.000002416529,0.0002122963,0.000003845124,0.00015780343],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994314,0.000004894037,0.000001913019,0.000014838267,0.000018742414,0.000016465083],"domain_scores_gemma":[0.9997987,0.000018773264,0.000059616377,0.00001537094,0.000019468807,0.000088084445],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000108238906,0.0001848764,0.00019889903,0.00076894736,0.00025592736,0.00035923114,0.00019739759,0.00019356074,0.000857343],"category_scores_gemma":[0.00016590538,0.00011791312,0.00019903808,0.00030774367,0.0002333825,0.0001874148,0.00046186443,0.00020822391,0.00022001527],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035461196,0.00010917984,0.7642509,0.000043178312,0.00015835144,0.0011347836,0.0009628726,0.0014732056,0.2168629,0.0005788538,0.0010637608,0.01300743],"study_design_scores_gemma":[0.0000042969177,0.000031189255,0.9976776,0.000002625631,0.000009665409,0.000082474064,0.000064883156,0.0005475916,0.0012218718,0.000031539126,0.00032261186,0.000003579153],"about_ca_topic_score_codex":0.01048552,"about_ca_topic_score_gemma":0.01390795,"teacher_disagreement_score":0.01048552,"about_ca_system_score_codex":0.00035002557,"about_ca_system_score_gemma":0.00015166972,"threshold_uncertainty_score":0.02084899},"labels":[],"label_agreement":null},{"id":"W4407420641","doi":"10.3847/1538-4357/adad66","title":"ASKAP Observations of the Radio Shell in the Composite Supernova Remnant G310.6-1.6","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Government of Western Australia; Ministry of Science and Technology of the People's Republic of China; Yunnan University; National Natural Science Foundation of China; Canada Research Chairs; Australian Government; Commonwealth Scientific and Industrial Research Organisation; Science and Industry Endowment Fund","keywords":"Physics; Astrophysics; Shell (structure); Supernova; Supernova remnant; Composite number; Astronomy; Composite material","score_opus":0.012961544571465311,"score_gpt":0.22810492963609053,"score_spread":0.21514338506462521,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407420641","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980919,0.00007341787,0.00030618507,0.000019631954,0.0000028051095,0.000005018875,0.00040211302,0.000029027486,0.0010698269],"genre_scores_gemma":[0.9980994,0.000037276186,0.0007718198,0.000017735905,0.0000052524824,0.000005371322,0.0007437853,0.0000075542903,0.0003118883],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993813,0.000006344216,0.0000037022571,0.000015205288,0.000023636205,0.000012972623],"domain_scores_gemma":[0.99976045,0.00002520972,0.00006854699,0.000028136727,0.000039672334,0.000077954275],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026635441,0.00015745849,0.0001698703,0.0008204452,0.00032089674,0.00022920035,0.0002688271,0.00025741672,0.0008115275],"category_scores_gemma":[0.00025734285,0.00014704974,0.00019043729,0.0004153718,0.00013667552,0.00015183412,0.00039834314,0.0002028258,0.00034083542],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008809691,0.00012292876,0.6632396,0.00005669472,0.000121437624,0.0019149923,0.00029824523,0.001303669,0.31696996,0.00046205174,0.0010260735,0.013603363],"study_design_scores_gemma":[0.000007363605,0.00004901307,0.9950506,0.0000022621218,0.000013851931,0.00041717425,0.000030848983,0.00083623285,0.0030286927,0.000063193904,0.00049579685,0.0000049025152],"about_ca_topic_score_codex":0.0019351018,"about_ca_topic_score_gemma":0.003734228,"teacher_disagreement_score":0.0019351018,"about_ca_system_score_codex":0.00015503795,"about_ca_system_score_gemma":0.00007109624,"threshold_uncertainty_score":0.0038477182},"labels":[],"label_agreement":null},{"id":"W4407556678","doi":"10.3847/1538-4357/adad6a","title":"Exploring the Key Features of Repeating Fast Radio Bursts with Machine Learning","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"National Natural Science Foundation of China","keywords":"Physics; Key (lock); Astronomy; Astrophysics; Computer security","score_opus":0.015173057214136625,"score_gpt":0.21901882689184274,"score_spread":0.20384576967770612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407556678","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88205504,0.0006633657,0.11312343,0.0003221156,0.000050979266,0.000065892214,0.00065832766,0.0008691251,0.002191598],"genre_scores_gemma":[0.96550035,0.00010869727,0.03239831,0.00003915696,0.000035724428,0.000023901906,0.0012411746,0.000028126586,0.0006244957],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9997633,0.00005948779,0.00001509002,0.00007174775,0.000052734078,0.00003761467],"domain_scores_gemma":[0.99899465,0.00041779075,0.00020314481,0.0001175138,0.00019430667,0.00007253941],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007788801,0.00050164195,0.000311406,0.0015541265,0.00035742676,0.0008271568,0.0005572158,0.00042189794,0.00081496517],"category_scores_gemma":[0.002064909,0.00011684144,0.00040761626,0.0009066617,0.00025572418,0.0006431393,0.00041067277,0.00051409024,0.00043981423],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002737362,0.00048299643,0.3636796,0.00016346909,0.00021443192,0.00026132053,0.00024910123,0.14157401,0.025390439,0.0020015524,0.0059815524,0.45972773],"study_design_scores_gemma":[0.000008004243,0.00004300288,0.0482763,0.0000144424275,0.000026516615,0.00004469367,0.000102652164,0.94631857,0.0025165128,0.0017453622,0.0008885821,0.000015329408],"about_ca_topic_score_codex":0.003928807,"about_ca_topic_score_gemma":0.004019692,"teacher_disagreement_score":0.003928807,"about_ca_system_score_codex":0.00024995714,"about_ca_system_score_gemma":0.00036349252,"threshold_uncertainty_score":0.007811904},"labels":[],"label_agreement":null},{"id":"W4407582587","doi":"10.3847/1538-4357/ad9749","title":"Swift-BAT GUANO Follow-up of Gravitational-wave Triggers in the Third LIGO–Virgo–KAGRA Observing Run","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"European Social Fund; Japan Society for the Promotion of Science; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; Science and Technology Facilities Council; National Science and Technology Council; European Regional Development Fund; Centre National de la Recherche Scientifique; ICTP South American Institute for Fundamental Research; Ministry of Science and ICT, South Korea; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; National Research Foundation; Vlaamse regering; National Astronomical Observatory of Japan; Ministry of Education, Culture, Sports, Science and Technology; Natural Sciences and Engineering Research Council of Canada; Ministry of Education, India; Agencia Estatal de Investigación; Great Southern Development Commission, Government of Western Australia; Israel Science Foundation; Scottish Universities Physics Alliance; National Natural Science Foundation of China; National Research Foundation of Korea; Division of Human Resource Development; Korea Astronomy and Space Science Institute; Nuclear Safety and Security Commission; Hungarian Scientific Research Fund; Generalitat de Catalunya; Generalitat Valenciana; Istituto Nazionale di Fisica Nucleare; U.S. Department of Energy; National Research, Development and Innovation Office; Korea Institute of Science and Technology Information; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Council of Scientific and Industrial Research, India; Fundacja na rzecz Nauki Polskiej; Academia Sinica; Abdus Salam International Centre for Theoretical Physics; Leverhulme Trust; European Commission; Russian Science Foundation; Scottish Funding Council; Narodowa Agencja Wymiany Akademickiej; Centres de Recerca de Catalunya; Institut des Origines de Lyon; Fonds De La Recherche Scientifique - FNRS; Fonds Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; Science and Engineering Research Board; National Science Foundation","keywords":"Physics; LIGO; Swift; Astrophysics; Gravitational wave; Astronomy; Neutron star; Telescope; Sky","score_opus":0.020322139536350266,"score_gpt":0.31401317137132156,"score_spread":0.2936910318349713,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407582587","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99648225,0.000037953247,0.000582229,0.00003463082,0.000005869644,0.000016535525,0.0018510709,0.00015502234,0.00083445676],"genre_scores_gemma":[0.99318475,0.000016370557,0.00090521167,0.000022763757,0.000007738769,0.000016869031,0.0054929685,0.00005749372,0.00029588077],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996458,0.00003833764,0.000013308476,0.0000925698,0.00009728814,0.00011271691],"domain_scores_gemma":[0.9983741,0.00027031757,0.0005087984,0.00022302273,0.00021586625,0.00040779263],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005994344,0.00022693255,0.00036657086,0.0007987014,0.00043157843,0.0006989714,0.00026410082,0.0003036741,0.0010678642],"category_scores_gemma":[0.0016062366,0.00012513582,0.00032935172,0.0007399201,0.00023794838,0.00022901532,0.0008785044,0.00043464004,0.000384663],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00091940025,0.00014142782,0.9646492,0.00003496104,0.0001235505,0.000588649,0.00041118675,0.0029482443,0.013043731,0.00037767264,0.0025313292,0.01423061],"study_design_scores_gemma":[0.00002544948,0.00008157592,0.9902879,0.000007316404,0.000036640366,0.00014812131,0.000121612116,0.0058762454,0.0020596317,0.00012610397,0.0012153729,0.000014035639],"about_ca_topic_score_codex":0.013882208,"about_ca_topic_score_gemma":0.028198797,"teacher_disagreement_score":0.013882208,"about_ca_system_score_codex":0.00037545955,"about_ca_system_score_gemma":0.0004898104,"threshold_uncertainty_score":0.027602851},"labels":[],"label_agreement":null},{"id":"W4407757190","doi":"10.3847/1538-4357/adae8d","title":"Influence of Modeling Assumptions on the Inferred Dynamical State of Resonant Systems: A Case Study of the HD 45364 System","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Institute for Theoretical Astrophysics","keywords":"Physics; Statistical physics; State (computer science); Dynamical systems theory; Astrophysics; Astronomy; Quantum mechanics; Algorithm","score_opus":0.01584804557251272,"score_gpt":0.25103155952778994,"score_spread":0.23518351395527723,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407757190","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973425,0.00006269192,0.0015130397,0.00013467095,0.000003998709,0.00001291895,0.00018833272,0.000042827796,0.00069891755],"genre_scores_gemma":[0.99866784,0.000021666647,0.0010725514,0.000010820464,0.000006546103,0.0000048157085,0.00013895519,0.00000923632,0.00006757195],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9990785,0.0005578664,0.000059205173,0.00016464196,0.000068847345,0.00007090217],"domain_scores_gemma":[0.98571914,0.012048969,0.0007922125,0.00075544877,0.0004387845,0.00024537713],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0036108252,0.0006012927,0.000551118,0.00096026505,0.001014067,0.0012820543,0.0012914349,0.0010255998,0.00095838535],"category_scores_gemma":[0.013570254,0.0003782964,0.00090400607,0.0006565208,0.0008640676,0.0011971085,0.0008763415,0.000929253,0.00012908108],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045669952,0.0001967005,0.18158051,0.000083935716,0.00018937406,0.0010339093,0.00047981893,0.8037468,0.002037646,0.0026849068,0.0005632778,0.0069464575],"study_design_scores_gemma":[0.00005831425,0.0000802361,0.02789832,0.000018294126,0.00005570204,0.000118927834,0.00024565362,0.9687752,0.0009255191,0.0013058598,0.00048843806,0.00002955941],"about_ca_topic_score_codex":0.045203563,"about_ca_topic_score_gemma":0.027368143,"teacher_disagreement_score":0.045203563,"about_ca_system_score_codex":0.00222723,"about_ca_system_score_gemma":0.00066525524,"threshold_uncertainty_score":0.08988088},"labels":[],"label_agreement":null},{"id":"W4407797391","doi":"10.3847/1538-4357/adabe7","title":"Evidence for Jet/Outflow Shocks Heating the Environment around the Class I Protostellar Source Elias 29: FAUST XXI","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Planetary Science Division; National Institutes of Natural Sciences; Science and Technology Facilities Council; HORIZON EUROPE Framework Programme; Ministerio de Ciencia e Innovación; Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Natural Sciences and Engineering Research Council of Canada; National Science Council; National Astronomical Observatory of Japan; European Regional Development Fund; European Commission; Japan Society for the Promotion of Science; Horizon 2020 Framework Programme; Deutsche Forschungsgemeinschaft; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Agencia Estatal de Investigación; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; FAUST; Outflow; Jet (fluid); Astrophysics; Astronomy; Protostar; Class (philosophy); Stars; Mechanics; Star formation; Meteorology; History; Art history","score_opus":0.027543535487923865,"score_gpt":0.27516966065953236,"score_spread":0.24762612517160848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407797391","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998264,0.000038942617,0.00019718047,0.00003653331,0.000002187033,0.0000041492344,0.00021338335,0.0000850851,0.0011585839],"genre_scores_gemma":[0.99914515,0.000018947596,0.00020157239,0.000023042985,0.0000034417071,0.0000029745127,0.00026818897,0.00001696674,0.00031972028],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996865,0.0000023484997,9.527843e-7,0.000010034146,0.0000062499457,0.000011799414],"domain_scores_gemma":[0.9998659,0.000014171106,0.00005305094,0.00001476985,0.000012518522,0.000039608618],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000057819743,0.00018551773,0.00014291958,0.0002525869,0.00032007942,0.00038609136,0.00023228384,0.00019552028,0.0013516685],"category_scores_gemma":[0.00013375362,0.00012221957,0.00011703245,0.00014709996,0.00021050799,0.000099835444,0.0003504787,0.00026490304,0.00027721756],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005548295,0.00015839231,0.6137179,0.00005966822,0.00009521596,0.0024247074,0.00056232634,0.0033181733,0.36443174,0.0006111273,0.002414066,0.011651773],"study_design_scores_gemma":[0.000025012654,0.00007342715,0.9845902,0.000009584349,0.000019637564,0.00034494672,0.00019609876,0.0025420825,0.010116262,0.0000855993,0.0019875108,0.000009707403],"about_ca_topic_score_codex":0.0053860387,"about_ca_topic_score_gemma":0.0051356335,"teacher_disagreement_score":0.0053860387,"about_ca_system_score_codex":0.00034562568,"about_ca_system_score_gemma":0.00012663049,"threshold_uncertainty_score":0.010709345},"labels":[],"label_agreement":null},{"id":"W4407798673","doi":"10.3847/1538-4357/adae10","title":"Fast and Efficient Bayesian Method to Search for Strongly Lensed Gravitational Waves","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Department of Atomic Energy, Government of India; Tata Institute of Fundamental Research","keywords":"Physics; Gravitational wave; Bayesian probability; Astrophysics; Astronomy; Gravitation; Artificial intelligence","score_opus":0.013522328091715066,"score_gpt":0.36017305720887804,"score_spread":0.346650729117163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407798673","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.011767169,0.000114676914,0.9858298,0.00013861146,0.00002308764,0.000070917304,0.00016678966,0.0008907273,0.0009982924],"genre_scores_gemma":[0.17253424,0.0001436677,0.8202469,0.00019197108,0.00015616576,0.00030484234,0.0017344373,0.00043464085,0.004253187],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99834013,0.0005343568,0.000082896724,0.00023040181,0.00061857206,0.00019356702],"domain_scores_gemma":[0.9949981,0.0032077662,0.00034536843,0.00038698656,0.00081842276,0.00024333538],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0031833155,0.00105827,0.0015470284,0.0024616753,0.0009898028,0.0016197228,0.0029669278,0.0015412464,0.009155731],"category_scores_gemma":[0.012505607,0.0011723237,0.0011864167,0.0015440191,0.00079134636,0.0019428503,0.0027262657,0.0017829855,0.0021299082],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007981297,0.00030881428,0.008130472,0.00023505992,0.00031489608,0.00036182307,0.000259573,0.4743327,0.0068082456,0.07106644,0.009244504,0.42813927],"study_design_scores_gemma":[0.000028759427,0.000014467575,0.0003582664,0.000009262225,0.000010578428,0.00003545285,0.000014205009,0.9868615,0.00053334516,0.011189203,0.0009323606,0.000012669151],"about_ca_topic_score_codex":0.011778608,"about_ca_topic_score_gemma":0.015457238,"teacher_disagreement_score":0.011778608,"about_ca_system_score_codex":0.0009661226,"about_ca_system_score_gemma":0.0033757302,"threshold_uncertainty_score":0.03062892},"labels":[],"label_agreement":null},{"id":"W4407925016","doi":"10.3847/1538-4357/adaf8d","title":"A Very Long Baseline Interferometry Calibrator Grid at 600 MHz for Fast Radio Transient Localizations with CHIME/FRB Outriggers","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Interferometry; Transient (computer programming); Astrophysics; Radio telescope; Astronomy","score_opus":0.005983358033810343,"score_gpt":0.21813719249479702,"score_spread":0.21215383446098668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4407925016","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.88105774,0.0005288004,0.06332181,0.0002457793,0.00006606889,0.00074975466,0.029439406,0.008709126,0.015881589],"genre_scores_gemma":[0.8326329,0.00013184463,0.11463707,0.00014849895,0.000038806007,0.00036508014,0.04713179,0.0008007217,0.004113326],"study_design_codex":"observational","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.9990497,0.00010392059,0.0000345392,0.00031803577,0.0002706628,0.00022306088],"domain_scores_gemma":[0.99673283,0.0002319611,0.00043286057,0.001285026,0.00066941726,0.0006479159],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.001576029,0.00034882367,0.00065879413,0.0021897794,0.0007574643,0.00062943547,0.0009369226,0.00041517665,0.0049261134],"category_scores_gemma":[0.0025752322,0.00038449306,0.00035938993,0.0029711723,0.00033574618,0.0005393053,0.0012909595,0.00045538167,0.002733056],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015211698,0.0005284603,0.52964586,0.00013079352,0.00013616426,0.000454048,0.0013508511,0.020251913,0.051202383,0.0014743205,0.031227557,0.3620765],"study_design_scores_gemma":[0.00020998807,0.00035196208,0.8835262,0.000046647972,0.000054077977,0.0002937558,0.00055697147,0.034859624,0.013468476,0.0006266085,0.06588903,0.00011670754],"about_ca_topic_score_codex":0.07310533,"about_ca_topic_score_gemma":0.13433398,"teacher_disagreement_score":0.07310533,"about_ca_system_score_codex":0.00079500873,"about_ca_system_score_gemma":0.0014846545,"threshold_uncertainty_score":0.14535964},"labels":[],"label_agreement":null},{"id":"W4408151743","doi":"10.3847/1538-4357/ada94b","title":"Search for Neutrino Emission from Hard X-Ray AGN with IceCube","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":35,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Alliance de recherche numérique du Canada; Santen; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Fonds Wetenschappelijk Onderzoek; Nvidia; Marquette University","keywords":"Physics; Astrophysics; Neutrino astronomy; Astronomy; Neutrino; Neutrino detector; Astroparticle physics; Cosmic ray; Neutrino oscillation; Nuclear physics","score_opus":0.010786644353361923,"score_gpt":0.2431107474696892,"score_spread":0.23232410311632726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408151743","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.93095684,0.000312352,0.0052774134,0.00026038158,0.00004649497,0.00013983474,0.040536232,0.002003277,0.020467103],"genre_scores_gemma":[0.8834826,0.00038713717,0.026008904,0.00026589652,0.00009220362,0.00024640167,0.08496753,0.0003660208,0.0041833627],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998148,0.000031344156,0.00001004522,0.000055596287,0.000054926513,0.000033360622],"domain_scores_gemma":[0.99949837,0.00011996426,0.0001429183,0.000085518026,0.00007699497,0.00007634721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005567197,0.00030846626,0.00029754825,0.0012331189,0.00025702605,0.00053963595,0.00034872344,0.00019321482,0.0031009275],"category_scores_gemma":[0.00059088215,0.00018683885,0.00037532157,0.0013437581,0.00011746535,0.000286578,0.00054279744,0.00022851366,0.00076231785],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0023972765,0.00034552498,0.7904483,0.0002661572,0.00059739064,0.0010630563,0.0006551955,0.010985647,0.06983915,0.0027306585,0.04859849,0.072073124],"study_design_scores_gemma":[0.00022141046,0.0003802373,0.79853183,0.000090110974,0.00027603004,0.0007260397,0.00047454116,0.050524306,0.047415826,0.0018233253,0.09949042,0.00004586513],"about_ca_topic_score_codex":0.004811088,"about_ca_topic_score_gemma":0.008048668,"teacher_disagreement_score":0.004811088,"about_ca_system_score_codex":0.00035574473,"about_ca_system_score_gemma":0.0002939137,"threshold_uncertainty_score":0.010373652},"labels":[],"label_agreement":null},{"id":"W4408157623","doi":"10.3847/1538-4357/adae0f","title":"Tracking X-Ray Variability in Next-generation EHT Low-luminosity Active Galactic Nucleus Targets","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Fonds de recherche du Québec – Nature et technologies; Natural Sciences and Engineering Research Council of Canada; National Aeronautics and Space Administration; California Institute of Technology; Agencia Nacional de Investigación y Desarrollo; Canada Research Chairs; McGill University","keywords":"Physics; Active galactic nucleus; Astrophysics; Luminosity; Nucleus; Tracking (education); Astronomy; Galaxy; Medicine","score_opus":0.02161069881840332,"score_gpt":0.25039224358574524,"score_spread":0.22878154476734192,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408157623","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978678,0.000046059267,0.0005105032,0.000019721494,0.0000017360417,0.0000076114675,0.00062126573,0.00008031116,0.0008449593],"genre_scores_gemma":[0.99668944,0.00001568861,0.0011483048,0.000014913435,0.000006842411,0.0000072554435,0.001841826,0.00001400699,0.00026168118],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999597,0.00006350613,0.000015578244,0.00011781488,0.00013153319,0.00007457767],"domain_scores_gemma":[0.9990169,0.000104941755,0.00031238882,0.00017230507,0.00019978247,0.00019368494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007625373,0.00014976527,0.00028127898,0.00069455296,0.0002778762,0.00066501333,0.00055359013,0.00019714572,0.0005302186],"category_scores_gemma":[0.0008406314,0.000120800214,0.00021872556,0.00034921296,0.0001485212,0.00032366044,0.00078772975,0.00020656642,0.0003053536],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002469105,0.000106456595,0.9670078,0.000017972621,0.00008814408,0.0002173515,0.00018080267,0.0026867408,0.017342098,0.00013200924,0.0006203693,0.011353361],"study_design_scores_gemma":[0.000011200057,0.00009623682,0.9891679,0.0000035167639,0.000023003675,0.00013949274,0.000059616257,0.006390495,0.0029434373,0.000027592645,0.0011309504,0.0000064410306],"about_ca_topic_score_codex":0.0099861575,"about_ca_topic_score_gemma":0.013436881,"teacher_disagreement_score":0.0099861575,"about_ca_system_score_codex":0.00052021176,"about_ca_system_score_gemma":0.0001267959,"threshold_uncertainty_score":0.019856095},"labels":[],"label_agreement":null},{"id":"W4408239288","doi":"10.3847/1538-4357/adb1de","title":"Observation of Cosmic-Ray Anisotropy in the Southern Hemisphere with 12 yr of Data Collected by the IceCube Neutrino Observatory","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"Office of Experimental Program to Stimulate Competitive Research; Deutsches Elektronen-Synchrotron; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Office of Advanced Cyberinfrastructure; Loyola University Chicago; Deutsche Forschungsgemeinschaft; Belgian Federal Science Policy Office; Bundesministerium für Bildung und Forschung; Michigan State University; Fonds Wetenschappelijk Onderzoek; Marquette University; University of Wisconsin-Madison; Office of Polar Programs; Fonds De La Recherche Scientifique - FNRS; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Cosmic ray; Northern Hemisphere; Neutrino; Muon; Astrophysics; Observatory; Anisotropy; Zenith; Monte Carlo method; Range (aeronautics); COSMIC cancer database; Astronomy; Southern Hemisphere; Nuclear physics; Statistics","score_opus":0.019095709613666002,"score_gpt":0.23363795331145326,"score_spread":0.21454224369778727,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408239288","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9924125,0.00021243017,0.0005951136,0.00004595163,0.0000121195735,0.000007791632,0.0053161206,0.000062977815,0.0013351089],"genre_scores_gemma":[0.9884239,0.00012684085,0.00072842604,0.0000138378755,0.00002616286,0.000013976005,0.010438631,0.00003415262,0.0001941947],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997434,0.00006198331,0.00001394206,0.000062766594,0.000064828535,0.000053082495],"domain_scores_gemma":[0.99903846,0.00017996361,0.00036157845,0.00015284389,0.00014575539,0.00012136671],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00081329566,0.00036242505,0.00039631553,0.0015441653,0.00029758853,0.00067805767,0.00020532048,0.00020021363,0.0008111259],"category_scores_gemma":[0.0012227981,0.00018844262,0.00041162944,0.0019107732,0.0002670407,0.0002489428,0.00058894773,0.00028558244,0.00022143623],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040322728,0.00007404364,0.9734972,0.00004566249,0.00023931917,0.00032569293,0.00014881136,0.005033851,0.008982249,0.00033880275,0.0016101621,0.009300963],"study_design_scores_gemma":[0.000009774202,0.000022240818,0.9940467,0.0000075891357,0.000024333362,0.0000949266,0.000036113186,0.0024715262,0.0011016598,0.00008393333,0.002092944,0.000008229628],"about_ca_topic_score_codex":0.008632156,"about_ca_topic_score_gemma":0.013178627,"teacher_disagreement_score":0.008632156,"about_ca_system_score_codex":0.00035927683,"about_ca_system_score_gemma":0.00030016413,"threshold_uncertainty_score":0.017163813},"labels":[],"label_agreement":null},{"id":"W4408246826","doi":"10.3847/1538-4357/adab71","title":"An In-depth Study of Gamma Rays from the Starburst Galaxy M82 with VERITAS","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Gamma ray; Gamma-ray astronomy","score_opus":0.007320525170346134,"score_gpt":0.2325242078759449,"score_spread":0.22520368270559876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408246826","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986512,0.0001732342,0.00023497177,0.000020141768,0.0000016805492,0.0000033344127,0.00017503287,0.000020234684,0.000720284],"genre_scores_gemma":[0.99828374,0.00009874316,0.0005587237,0.000023093797,0.000007750311,0.000002650424,0.00052089203,0.000016999367,0.0004874885],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985564,0.000019784651,0.000006850989,0.000039631937,0.00004527245,0.000032782795],"domain_scores_gemma":[0.9994863,0.00009451733,0.00016987811,0.00008463911,0.000103353676,0.000061227904],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032507334,0.00021908812,0.00021902024,0.0013198126,0.00029024523,0.0005487564,0.00027250824,0.00021728323,0.00096893276],"category_scores_gemma":[0.00044851843,0.00017647653,0.00019769256,0.0011611965,0.0002048623,0.00031569746,0.0005506308,0.00022905417,0.0002434707],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002644585,0.00008219502,0.79452205,0.00007528669,0.00010916668,0.0018168697,0.0016212071,0.0011865582,0.1713608,0.0004827462,0.0005422651,0.027936434],"study_design_scores_gemma":[0.000005196577,0.00008347297,0.990141,0.000009516393,0.0000275034,0.00056678505,0.00036752212,0.0014011532,0.0052447254,0.00009245909,0.002052453,0.00000811743],"about_ca_topic_score_codex":0.0049263844,"about_ca_topic_score_gemma":0.011736141,"teacher_disagreement_score":0.0049263844,"about_ca_system_score_codex":0.00032432575,"about_ca_system_score_gemma":0.00013684428,"threshold_uncertainty_score":0.009795427},"labels":[],"label_agreement":null},{"id":"W4408374712","doi":"10.3847/1538-4357/adb312","title":"Search for Neutrino Doublets and Triplets Using 11.4 yr of IceCube Data","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Alliance de recherche numérique du Canada; Santen; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Fonds Wetenschappelijk Onderzoek; Nvidia; Marquette University","keywords":"Physics; Neutrino; Nuclear physics","score_opus":0.03979069804330785,"score_gpt":0.3055077837964851,"score_spread":0.2657170857531772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408374712","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94152665,0.00093336013,0.009962722,0.00021902757,0.00006720552,0.00011586164,0.035948776,0.00087841804,0.010348005],"genre_scores_gemma":[0.88781106,0.000430299,0.023202179,0.00014414937,0.00009370366,0.00018220484,0.08444675,0.000274759,0.0034150332],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99933004,0.0001456188,0.00002909855,0.00021365687,0.00014078329,0.0001408765],"domain_scores_gemma":[0.99907565,0.00027875943,0.0002475633,0.00014281769,0.00013378622,0.00012144255],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014396384,0.000647692,0.00079654244,0.0018422086,0.00060697057,0.0011736215,0.00044540054,0.00045043,0.0038188596],"category_scores_gemma":[0.0010920948,0.0003099727,0.0010439528,0.0017710498,0.00019984494,0.0004235019,0.0007528146,0.00041732652,0.0011723383],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0065510175,0.0005407644,0.71524256,0.00056074554,0.0019425061,0.0013473529,0.00043187445,0.03209284,0.13428558,0.0036155512,0.01874517,0.084644],"study_design_scores_gemma":[0.00051229895,0.0008019128,0.72341543,0.00013404516,0.00092902494,0.0009916156,0.0004099103,0.09683691,0.083790995,0.0040995153,0.087913685,0.00016467438],"about_ca_topic_score_codex":0.0073565994,"about_ca_topic_score_gemma":0.011536886,"teacher_disagreement_score":0.0073565994,"about_ca_system_score_codex":0.00074400345,"about_ca_system_score_gemma":0.0008332505,"threshold_uncertainty_score":0.014627576},"labels":[],"label_agreement":null},{"id":"W4408581541","doi":"10.3847/1538-4357/adaec1","title":"The UNCOVER Survey: First Release of Ultradeep JWST/NIRSpec PRISM Spectra for ∼700 Galaxies from <i>z</i> ∼ 0.3–13 in A2744","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":42,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"Israel Science Foundation; United States-Israel Binational Science Foundation; Space Telescope Science Institute; National Research Foundation; University of Pittsburgh; Center for Research Computing, University of Pittsburgh; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Reionization; Redshift; Galaxy; Astrophysics; James Webb Space Telescope; Astronomy; Photometry (optics); Globular cluster; Population; Stars","score_opus":0.006566805628096527,"score_gpt":0.2113761415824632,"score_spread":0.20480933595436668,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408581541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9586859,0.00011080338,0.0020692933,0.0000821942,0.000010994001,0.00010267967,0.03441075,0.00062819966,0.0038992139],"genre_scores_gemma":[0.8109758,0.00018128812,0.020768609,0.0002724503,0.00006492503,0.00030835913,0.16091734,0.00039516162,0.006116028],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999627,0.000026433469,0.000021902228,0.00008555505,0.00014658613,0.00009251616],"domain_scores_gemma":[0.99873644,0.00007650102,0.00029121301,0.00027214465,0.00030361462,0.00032009368],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049431995,0.00025670032,0.0002545653,0.0016620696,0.0003230408,0.00044944911,0.0006396155,0.0001730428,0.0021819635],"category_scores_gemma":[0.0005224247,0.00032867544,0.000341169,0.0009249436,0.00014122686,0.00037353844,0.0009895567,0.00027237344,0.0009499979],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004900145,0.00030229022,0.83025724,0.00012301149,0.00015112241,0.0002673315,0.0007434332,0.0011863234,0.058110725,0.00028470863,0.019996792,0.08808704],"study_design_scores_gemma":[0.000021493834,0.00005880597,0.9889353,0.000006424083,0.000020768206,0.00008551437,0.000077199395,0.0006403421,0.002181506,0.000032215517,0.0079291295,0.000011270231],"about_ca_topic_score_codex":0.021230243,"about_ca_topic_score_gemma":0.055951294,"teacher_disagreement_score":0.021230243,"about_ca_system_score_codex":0.0004539655,"about_ca_system_score_gemma":0.00069899904,"threshold_uncertainty_score":0.04221338},"labels":[],"label_agreement":null},{"id":"W4408581865","doi":"10.3847/1538-4357/adb623","title":"Rare Event Classification with Weighted Logistic Regression for Identifying Repeating Fast Radio Bursts","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Anomaly Detection Techniques and Applications","field":"Computer Science","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Statistical Sciences Institute","keywords":"Physics; Logistic regression; Event (particle physics); Astrophysics; Astronomy; Pattern recognition (psychology); Artificial intelligence; Medicine; Internal medicine; Computer science","score_opus":0.032063333364822394,"score_gpt":0.31127479680912734,"score_spread":0.2792114634443049,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408581865","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.25994924,0.0010028835,0.7335061,0.00067496544,0.00015548652,0.00013676904,0.00070391624,0.0029102736,0.0009603811],"genre_scores_gemma":[0.8416727,0.00029876558,0.15369888,0.00013303808,0.00022003264,0.00014416515,0.0016803402,0.00023107081,0.00192102],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99729615,0.0013560947,0.00017631066,0.00059880514,0.00037614876,0.00019642539],"domain_scores_gemma":[0.985413,0.009999172,0.0018873881,0.001163,0.0012146711,0.0003227721],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.007238714,0.0012446494,0.0011811834,0.00406762,0.00052550016,0.0012044401,0.0025307622,0.0014122637,0.0018878363],"category_scores_gemma":[0.022380734,0.00040007127,0.0011595418,0.0022258752,0.00055468525,0.0016474318,0.0014024763,0.0019508166,0.0018121686],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010822944,0.00047223447,0.11355542,0.00027545966,0.00061204506,0.00075271376,0.00027086984,0.4269158,0.008590008,0.0033300407,0.006003739,0.43813935],"study_design_scores_gemma":[0.000011066653,0.000038975726,0.0037084648,0.000011040742,0.00001654564,0.00009121113,0.000028129685,0.9932909,0.00085542334,0.0015959297,0.00033627948,0.000015953134],"about_ca_topic_score_codex":0.0034582336,"about_ca_topic_score_gemma":0.002032269,"teacher_disagreement_score":0.007238714,"about_ca_system_score_codex":0.00048451687,"about_ca_system_score_gemma":0.0005754009,"threshold_uncertainty_score":0.038282454},"labels":[],"label_agreement":null},{"id":"W4408677386","doi":"10.3847/1538-4357/adb30c","title":"VERITAS and Multiwavelength Observations of the Blazar B3 2247+381 in Response to an IceCube Neutrino Alert","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Institute of Particle Physics","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Office of Science; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Alliance de recherche numérique du Canada; Chiba University; Santen; Knut och Alice Wallenbergs Stiftelse; Nuclear Safety and Security Commission; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Queen's University Belfast; Deutsches Elektronen-Synchrotron; National Energy Research Scientific Computing Center; Space Telescope Science Institute; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Queen's University; Polarforskningssekretariatet; National Research Foundation of Korea; Villum Fonden; Marquette University; Vetenskapsrådet; Smithsonian Institution; U.S. Department of Energy; University of Wisconsin-Madison; Fonds Wetenschappelijk Onderzoek; Nvidia; National Aeronautics and Space Administration; Office of Advanced Cyberinfrastructure; European Commission; National Research Foundation; Michigan State University; Barnard College","keywords":"Physics; Blazar; Neutrino; Astrophysics; Flux (metallurgy); Neutrino astronomy; Neutrino detector; Observatory; Active galactic nucleus; Astronomy; Gamma ray; Neutrino oscillation; Galaxy; Particle physics","score_opus":0.013120406614384154,"score_gpt":0.24506728252888954,"score_spread":0.23194687591450538,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408677386","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99625117,0.00008756405,0.00026233,0.000055701257,0.000012597486,0.000010503012,0.0012131758,0.000096161675,0.002010914],"genre_scores_gemma":[0.99581593,0.000053378222,0.0010594086,0.000036486384,0.000019996933,0.000014583807,0.0022919022,0.00003097062,0.0006773513],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998388,0.00001840468,0.000006827517,0.0000441678,0.00006376415,0.000028021532],"domain_scores_gemma":[0.99941707,0.00007070576,0.00028154932,0.000055385288,0.000068291585,0.000107080756],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032438082,0.00026218782,0.00027628432,0.0009671269,0.00039939772,0.0004662019,0.00031175537,0.00031863197,0.0015551345],"category_scores_gemma":[0.00047118717,0.00018380911,0.00025982872,0.00053449895,0.00016795179,0.00021785744,0.0004220009,0.0004273071,0.0002606321],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0021434405,0.00025715178,0.69626373,0.00013561327,0.0003786175,0.0015082302,0.00071861653,0.0028005063,0.26582325,0.00072086795,0.004050422,0.025199499],"study_design_scores_gemma":[0.000027882825,0.0001094702,0.98748255,0.00001015061,0.00003539149,0.00020437474,0.00009292059,0.002432351,0.007454541,0.00009039379,0.0020445026,0.00001559301],"about_ca_topic_score_codex":0.009384372,"about_ca_topic_score_gemma":0.028490946,"teacher_disagreement_score":0.009384372,"about_ca_system_score_codex":0.00055996096,"about_ca_system_score_gemma":0.0001861908,"threshold_uncertainty_score":0.018659472},"labels":[],"label_agreement":null},{"id":"W4408833067","doi":"10.3847/1538-4357/adae05","title":"Magnetic Field Structures In and Around Seyfert Galaxy Outflows","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Dirección General de Asuntos del Personal Académico, Universidad Nacional Autónoma de México; Jet Propulsion Laboratory; Natural Sciences and Engineering Research Council of Canada; Department of Atomic Energy, Government of India; Tata Institute of Fundamental Research; California Institute of Technology; National Aeronautics and Space Administration; National Radio Astronomy Observatory; National Science Foundation","keywords":"Physics; Galaxy; Astronomy; Astrophysics; Magnetic field; Field (mathematics)","score_opus":0.004453743602213095,"score_gpt":0.21282758406105537,"score_spread":0.20837384045884227,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408833067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995091,0.000040783227,0.00005733006,0.000004195903,6.928382e-7,0.000001080705,0.0000679748,0.0000062259,0.00031249924],"genre_scores_gemma":[0.99954456,0.000028991108,0.0000730742,0.0000032344215,0.0000041781745,0.0000010019197,0.0002091327,0.0000016272396,0.0001342243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996674,0.000003914788,0.0000020653283,0.000008334894,0.000006395188,0.000012501042],"domain_scores_gemma":[0.99979955,0.000021942746,0.00009461064,0.000009841857,0.00002285825,0.000051122643],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007234293,0.00014602108,0.0001305275,0.0011901831,0.000167789,0.0003446307,0.000091776856,0.00011950737,0.0010842449],"category_scores_gemma":[0.00021092729,0.00007011526,0.000067250076,0.0004119826,0.00018510745,0.00012817027,0.0002513068,0.000074237265,0.00019212304],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002415954,0.000036108097,0.91871554,0.000023928576,0.0000337447,0.00087044877,0.000559569,0.00020463263,0.07120719,0.000088454166,0.00014526951,0.007873594],"study_design_scores_gemma":[0.000002154088,0.000020684894,0.9989975,0.0000015561443,0.0000032082564,0.00019371997,0.00010258303,0.000071512324,0.0004626673,0.00001397424,0.0001295636,9.225558e-7],"about_ca_topic_score_codex":0.0014101451,"about_ca_topic_score_gemma":0.0019531101,"teacher_disagreement_score":0.0014101451,"about_ca_system_score_codex":0.0001160224,"about_ca_system_score_gemma":0.00004528199,"threshold_uncertainty_score":0.0036271214},"labels":[],"label_agreement":null},{"id":"W4408869339","doi":"10.3847/1538-4357/adb1da","title":"Metis Observations of Alfvénic Outflows Driven by Interchange Reconnection in a Pseudostreamer","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council; Agenzia Spaziale Italiana; Bundesministerium für Wirtschaft und Energie; Leverhulme Trust; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Magnetic reconnection; Astrophysics; Astronomy; Metis; Plasma; Nuclear physics","score_opus":0.01248795239169539,"score_gpt":0.24581180890942494,"score_spread":0.23332385651772955,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408869339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982515,0.00003821606,0.0004622279,0.000015161903,0.0000046663463,0.000005952988,0.00017732917,0.00007769474,0.00096731464],"genre_scores_gemma":[0.9989912,0.000019105664,0.0005162085,0.000005928636,0.0000060545854,0.0000033508998,0.00030531568,0.000009243681,0.0001436307],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99996245,0.0000037707491,0.0000013961956,0.000008287294,0.00001496435,0.000009011392],"domain_scores_gemma":[0.99990547,0.00001426776,0.000023423561,0.000012799714,0.000013939096,0.000029972449],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010531332,0.00016312978,0.0002676596,0.00038344416,0.00028479856,0.00030833602,0.00022789983,0.00027375767,0.0006995505],"category_scores_gemma":[0.00017377778,0.00011280286,0.00019083246,0.00025034187,0.0001485144,0.0001639039,0.00032728055,0.00029951066,0.00012446225],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018222277,0.00035453038,0.34670162,0.00012302448,0.00019795616,0.0039695655,0.0012142103,0.019742459,0.5937106,0.00076944655,0.001882437,0.029512055],"study_design_scores_gemma":[0.00007077382,0.0003731271,0.9388287,0.000013615673,0.0000295914,0.0005054983,0.00035280368,0.036393754,0.021251336,0.00019903375,0.0019643365,0.000017495411],"about_ca_topic_score_codex":0.0009968232,"about_ca_topic_score_gemma":0.0021258034,"teacher_disagreement_score":0.0009968232,"about_ca_system_score_codex":0.00017333544,"about_ca_system_score_gemma":0.00007429667,"threshold_uncertainty_score":0.0023402572},"labels":[],"label_agreement":null},{"id":"W4408875883","doi":"10.3847/1538-4357/adb8e3","title":"Improved Constraints on the Faraday Rotation toward Eight Fast Radio Bursts Using Dense Grids of Polarized Radio Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Agencia Estatal de Investigación; European Commission; European Regional Development Fund; Natural Sciences and Engineering Research Council of Canada; Institut Périmètre de physique théorique; University of Toronto; Government of Canada; Ministry of Colleges and Universities; Comunidad de Madrid; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Research Chairs; National Science Foundation","keywords":"Physics; Faraday effect; Astrophysics; Radio galaxy; Astronomy; Rotation (mathematics); Galaxy; Faraday cage; X-shaped radio galaxy; Radio astronomy; Magnetic field","score_opus":0.01572784074845472,"score_gpt":0.30074397172591344,"score_spread":0.2850161309774587,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408875883","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9828042,0.00008157014,0.015118237,0.000053197797,0.000007120033,0.0000074229633,0.00058869855,0.00015267398,0.0011867792],"genre_scores_gemma":[0.99258184,0.000029716513,0.006461477,0.000015125272,0.00001713738,0.0000068462855,0.00078172656,0.000017961636,0.000088121546],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979824,0.000056488378,0.000008769644,0.00005817927,0.00004168478,0.000036541194],"domain_scores_gemma":[0.9985739,0.00045832235,0.00033787658,0.00031348979,0.00016981515,0.00014655241],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060373556,0.00030464525,0.00035857252,0.0010225358,0.00025589467,0.00078027043,0.00039487175,0.00020956036,0.0011270891],"category_scores_gemma":[0.0023398518,0.00042327767,0.00028437856,0.00055079925,0.0002698792,0.00027493655,0.000752745,0.0003407667,0.00033474067],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003700928,0.00013187811,0.84396535,0.000045980298,0.00017173252,0.00013576029,0.00024671794,0.084763534,0.028009284,0.0021493842,0.0014998975,0.038510464],"study_design_scores_gemma":[0.00013721202,0.00008314009,0.77877164,0.000037969567,0.00006922641,0.00012092417,0.00016424275,0.21033306,0.0033178169,0.0040490157,0.0028615135,0.000054284425],"about_ca_topic_score_codex":0.0048930617,"about_ca_topic_score_gemma":0.0069700633,"teacher_disagreement_score":0.0048930617,"about_ca_system_score_codex":0.00025023898,"about_ca_system_score_gemma":0.00022491376,"threshold_uncertainty_score":0.009729147},"labels":[],"label_agreement":null},{"id":"W4408875984","doi":"10.3847/1538-4357/adbbcb","title":"Bias-corrected Fast Radio Burst Population and Spectra Using CHIME Injection Data","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; Spectral line; Population; Astronomy","score_opus":0.03157225030449156,"score_gpt":0.34337435172697994,"score_spread":0.3118021014224884,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408875984","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96038693,0.00013922411,0.03195542,0.00006247139,0.000029112965,0.000056044402,0.0038660353,0.0012354058,0.0022693917],"genre_scores_gemma":[0.96967536,0.00006626435,0.02099487,0.00003756099,0.000012846126,0.000036231555,0.008231018,0.00020658584,0.0007392771],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99968314,0.000031077965,0.000016479118,0.00010090736,0.00011746925,0.000050993163],"domain_scores_gemma":[0.99899656,0.00019432152,0.000171178,0.00022684928,0.00036775199,0.000043395972],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00076568,0.00027037913,0.00018733404,0.0009846246,0.0002943961,0.00048029496,0.00043895558,0.0002796353,0.0009910587],"category_scores_gemma":[0.002519403,0.00016119373,0.00036731965,0.0011032962,0.00017153163,0.00039749173,0.00025307576,0.00032096283,0.00035651118],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029994082,0.00012524505,0.8321864,0.0000844252,0.000250388,0.00025110034,0.00026037102,0.03552333,0.040649064,0.001714144,0.0022555809,0.08639997],"study_design_scores_gemma":[0.000027886812,0.000052054773,0.7999676,0.000016245427,0.00011273197,0.00017242998,0.00009126109,0.16824314,0.023695575,0.00081425585,0.0067482227,0.000058635025],"about_ca_topic_score_codex":0.02673078,"about_ca_topic_score_gemma":0.035436302,"teacher_disagreement_score":0.02673078,"about_ca_system_score_codex":0.00079826306,"about_ca_system_score_gemma":0.000552594,"threshold_uncertainty_score":0.053150356},"labels":[],"label_agreement":null},{"id":"W4408881577","doi":"10.3847/1538-4357/adb8cd","title":"A 34 yr Timing Solution of the Redback Millisecond Pulsar Terzan 5A","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Australian Government; Canadian Institute for Advanced Research; National Aeronautics and Space Administration; Commonwealth Scientific and Industrial Research Organisation; National Science Foundation","keywords":"Physics; Millisecond pulsar; Astrophysics; Pulsar; Astronomy; Globular cluster; Millisecond; Neutron star; Stars","score_opus":0.01313474653819755,"score_gpt":0.3114908068986388,"score_spread":0.2983560603604412,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4408881577","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9491402,0.00059361546,0.03472564,0.00043660856,0.0003688606,0.00006829139,0.00395082,0.0010740646,0.009641884],"genre_scores_gemma":[0.94011766,0.00022821521,0.046023607,0.00010271586,0.00012711542,0.00004499197,0.0099260835,0.00017814114,0.0032514748],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.9998827,0.000013743672,0.0000087372255,0.000030246994,0.00004206923,0.000022501852],"domain_scores_gemma":[0.99969673,0.00003251559,0.00009791945,0.00003514101,0.000077550176,0.00006007685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030902936,0.00028617145,0.00027614762,0.001323594,0.00042435213,0.0005714734,0.0003693908,0.0003825398,0.0033086434],"category_scores_gemma":[0.00091167644,0.00016359381,0.00034422893,0.00069339795,0.000079990765,0.00026229233,0.00054071256,0.0005829483,0.0007436855],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010653659,0.0006054696,0.27698654,0.0003543082,0.0005266741,0.004535151,0.0011448002,0.07701293,0.230972,0.00828847,0.016879374,0.38162887],"study_design_scores_gemma":[0.00030914016,0.0010935081,0.7322466,0.00011717982,0.0002839826,0.001965574,0.0007087879,0.13631438,0.028741358,0.0036980133,0.094359234,0.0001622988],"about_ca_topic_score_codex":0.0023813772,"about_ca_topic_score_gemma":0.0041813403,"teacher_disagreement_score":0.0033086434,"about_ca_system_score_codex":0.0003021565,"about_ca_system_score_gemma":0.00038058666,"threshold_uncertainty_score":0.011068523},"labels":[],"label_agreement":null},{"id":"W4409037750","doi":"10.3847/1538-4357/adbd3a","title":"The Emerging Class of Double-faced White Dwarfs","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; Canadian Institute for Theoretical Astrophysics; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Smithsonian Institution; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; White dwarf; Class (philosophy); Astrophysics; Astronomy; Stars; Artificial intelligence","score_opus":0.00939750412350693,"score_gpt":0.2436770898464825,"score_spread":0.23427958572297558,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409037750","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99742186,0.00022235724,0.00068135984,0.00002291649,0.0000074395684,0.0000070509677,0.00018707133,0.000025166657,0.001424726],"genre_scores_gemma":[0.9979741,0.000076900644,0.0008757502,0.00003284146,0.000013370034,0.0000042590796,0.00045290758,0.000006570103,0.000563404],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99973863,0.000011117891,0.000015582636,0.00009239749,0.00008055126,0.000061710925],"domain_scores_gemma":[0.99934083,0.00005411529,0.00024470856,0.000056067016,0.00009386128,0.0002103836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001997059,0.00027652358,0.00035563827,0.00093560776,0.0005671062,0.00079059415,0.0003634643,0.00016868493,0.0014270765],"category_scores_gemma":[0.00043714372,0.00010587629,0.0001672365,0.00069649087,0.0003335003,0.00031012643,0.0010600272,0.00025941906,0.00049108366],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017286823,0.00005598114,0.91074765,0.000071769275,0.00006178284,0.001355311,0.00062445935,0.00017261569,0.04609467,0.0013384108,0.0006405227,0.038663805],"study_design_scores_gemma":[0.000009228296,0.00016148714,0.9775647,0.000020299689,0.00002852596,0.005505738,0.0007342009,0.00048905646,0.006233139,0.0008887102,0.008354283,0.000010750333],"about_ca_topic_score_codex":0.0007049459,"about_ca_topic_score_gemma":0.00140386,"teacher_disagreement_score":0.0014270765,"about_ca_system_score_codex":0.00016234693,"about_ca_system_score_gemma":0.00019959091,"threshold_uncertainty_score":0.0047740936},"labels":[],"label_agreement":null},{"id":"W4409128615","doi":"10.3847/1538-4357/ada608","title":"EPOCHS. I. The Discovery and Star-forming Properties of Galaxies in the Epoch of Reionization at 6.5 &lt; <i>z</i> &lt; 18 with PEARLS and Public JWST Data","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":19,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Reionization; Physics; Astrophysics; Galaxy; Epoch (astronomy); Astronomy; Star formation; Intergalactic medium; Star (game theory); Redshift","score_opus":0.015964476437768823,"score_gpt":0.2116536332108627,"score_spread":0.19568915677309387,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409128615","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9930455,0.00006745373,0.0003016368,0.00004059731,0.000003875421,0.000013659303,0.0047784876,0.0000991813,0.0016495541],"genre_scores_gemma":[0.99024487,0.00006320267,0.0007247518,0.000029627017,0.000015555494,0.000011535292,0.0076318705,0.000026706955,0.001251833],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998254,0.000009801768,0.000015115906,0.000043402004,0.00006036101,0.000045923694],"domain_scores_gemma":[0.9988807,0.000072560615,0.0005983232,0.0001315854,0.000111238005,0.00020558792],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003039997,0.00018961236,0.00015125956,0.0016373915,0.00019681444,0.00061119144,0.00025092324,0.00013451079,0.002446756],"category_scores_gemma":[0.0009374111,0.00013401329,0.00027114968,0.00081092067,0.0002574879,0.0006716605,0.000654916,0.00023020076,0.0005810966],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00007017311,0.000020854446,0.98677814,0.000017306364,0.000026410353,0.00012892294,0.0001767262,0.00022925975,0.004153179,0.00014202381,0.0014045628,0.0068525695],"study_design_scores_gemma":[0.0000022583095,0.000011704859,0.99784946,0.0000022402778,0.0000057702277,0.0001151068,0.00004125694,0.00021507159,0.0007907433,0.000026499341,0.00093817164,0.0000017346395],"about_ca_topic_score_codex":0.0036963706,"about_ca_topic_score_gemma":0.0072694914,"teacher_disagreement_score":0.0036963706,"about_ca_system_score_codex":0.00022931116,"about_ca_system_score_gemma":0.00009578348,"threshold_uncertainty_score":0.008185267},"labels":[],"label_agreement":null},{"id":"W4409128711","doi":"10.3847/1538-4357/adb620","title":"Eight Years of Light from ASASSN-15oi: Toward Understanding the Late-time Evolution of TDEs","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Astronomy","score_opus":0.012835417404565883,"score_gpt":0.22280309585926006,"score_spread":0.20996767845469416,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409128711","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973943,0.0002093995,0.00035834417,0.000040934225,0.000009152641,0.000007545585,0.0010006364,0.00001585296,0.00096373656],"genre_scores_gemma":[0.9964193,0.00010898914,0.00059110834,0.000055951274,0.000019423087,0.000010824751,0.0023882377,0.000011219362,0.00039490894],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999,0.0000103673665,0.0000063090647,0.000034004595,0.00002057705,0.000028690698],"domain_scores_gemma":[0.9995821,0.00003729555,0.00012525459,0.000046243145,0.00007912277,0.00013002673],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00044353947,0.00022899348,0.00030093122,0.0006607046,0.00036748007,0.00058651937,0.00022861062,0.00022158555,0.00069698546],"category_scores_gemma":[0.00042258462,0.00011846084,0.0002540079,0.0005150052,0.00018276332,0.0003188061,0.0006889301,0.00038703645,0.0002231592],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000108180386,0.000046135927,0.97668195,0.00002731381,0.00006599685,0.00014914977,0.00034286504,0.00035538635,0.01380489,0.00012766595,0.0004408682,0.007849422],"study_design_scores_gemma":[0.0000014937449,0.000026310954,0.99789125,0.0000067758224,0.00001094625,0.00004450082,0.00014951659,0.00033618076,0.00038290356,0.000045592333,0.0011013676,0.0000032897367],"about_ca_topic_score_codex":0.007938242,"about_ca_topic_score_gemma":0.02323819,"teacher_disagreement_score":0.007938242,"about_ca_system_score_codex":0.00036797347,"about_ca_system_score_gemma":0.0001852176,"threshold_uncertainty_score":0.015784085},"labels":[],"label_agreement":null},{"id":"W4409128960","doi":"10.3847/1538-4357/adb7df","title":"Detection of Molecular Clouds in the PeVatron Candidate Source LHAASO J0341+5258 by the Nobeyama 45-m Radio Telescope","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"Japan Society for the Promotion of Science","keywords":"Physics; Astronomy; Astrophysics; Telescope; Radio telescope","score_opus":0.0029589384425025888,"score_gpt":0.20553085337199206,"score_spread":0.20257191492948948,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409128960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99508345,0.00012563361,0.00030464446,0.000074194766,0.000009087052,0.000012876124,0.0004577575,0.000048828064,0.003883528],"genre_scores_gemma":[0.9974929,0.00005752765,0.00053939887,0.0000775822,0.000015633901,0.000016388469,0.0008876467,0.000015971988,0.0008970134],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999869,0.000008132995,0.000005592153,0.000036963585,0.00003562834,0.00004465127],"domain_scores_gemma":[0.9996432,0.000026934113,0.00008351485,0.00005149521,0.00006461324,0.00013024865],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015500838,0.0001899779,0.0002026296,0.00073069375,0.000588613,0.00061057456,0.00030734725,0.00032531735,0.00287227],"category_scores_gemma":[0.00031109326,0.00021435323,0.00017845567,0.00049464026,0.00020833948,0.0002343576,0.00063960033,0.00027312938,0.0006500692],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036583794,0.00016532619,0.7934489,0.00007707866,0.000113657145,0.0010119565,0.0007941233,0.00041113928,0.18034278,0.000247311,0.002117873,0.020903884],"study_design_scores_gemma":[0.00001890005,0.00006658124,0.993676,0.0000087487215,0.000035208293,0.00015124216,0.00026892315,0.00044357215,0.0022092205,0.000032036638,0.003081354,0.000008154861],"about_ca_topic_score_codex":0.013671732,"about_ca_topic_score_gemma":0.031749416,"teacher_disagreement_score":0.013671732,"about_ca_system_score_codex":0.00037914194,"about_ca_system_score_gemma":0.00024606858,"threshold_uncertainty_score":0.027184308},"labels":[],"label_agreement":null},{"id":"W4409129025","doi":"10.3847/1538-4357/adb974","title":"AT 2020nov: Evidence for Disk Reprocessing in a Rare Tidal Disruption Event","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Planetary Science Division; Institut National de Physique Nucléaire et de Physique des Particules; Science and Technology Facilities Council; Smithsonian Astrophysical Observatory; University of North Carolina at Chapel Hill; Max-Planck-Institut für Astronomie; Eötvös Loránd Tudományegyetem; PAZY Foundation; University of California, Los Angeles; Stockholms Universitet; Nuclear Safety and Security Commission; Science Mission Directorate; University of Toronto; Ministério da Ciência, Tecnologia e Inovação; Queen's University; Canada Research Chairs; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; Deutsches Elektronen-Synchrotron; United States-Israel Binational Science Foundation; Gordon and Betty Moore Foundation; Queen's University Belfast; National Science Foundation; UK Research and Innovation; National Central University; Villum Fonden; Los Alamos National Laboratory; College of Engineering, Michigan State University; University of Washington; Johns Hopkins University; Illinois Space Grant Consortium; NASA Exoplanet Science Institute; Jet Propulsion Laboratory; University of California, Santa Cruz; Heising-Simons Foundation; Space Telescope Science Institute; W. M. Keck Foundation; European Commission; California Institute of Technology; National Aeronautics and Space Administration; David and Lucile Packard Foundation; National Centre for Supercomputing Applications; University of Illinois at Urbana-Champaign; Michigan State University; Trinity College Dublin; Natural Sciences and Engineering Research Council of Canada; Durham University; Smithsonian Institution","keywords":"Physics; Event (particle physics); Astrophysics; Astronomy; Astrobiology","score_opus":0.023368011028478748,"score_gpt":0.31179757655622725,"score_spread":0.2884295655277485,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409129025","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99466586,0.0001154822,0.0004960464,0.000038466595,0.000009068941,0.000015479842,0.0012925187,0.00006391676,0.0033032484],"genre_scores_gemma":[0.9964503,0.00003601662,0.00030494397,0.00002142123,0.0000102117665,0.0000047018966,0.0021946921,0.000011373345,0.0009663246],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997764,0.000015270996,0.000019665444,0.000039623963,0.00007454127,0.00007448116],"domain_scores_gemma":[0.9991277,0.00007917811,0.00022827262,0.00009474437,0.00014590051,0.00032417424],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022010884,0.00021769422,0.00023449596,0.001303443,0.0004673603,0.00073473074,0.0003000414,0.00042452506,0.0022009632],"category_scores_gemma":[0.00074111,0.0001140867,0.0002974232,0.000750472,0.00023548448,0.00028042585,0.00076731725,0.00026983858,0.0008278839],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049362367,0.00008466089,0.95799166,0.000043087417,0.00004521004,0.003198549,0.00034008457,0.00068365165,0.024569225,0.0005732282,0.0011316137,0.01084532],"study_design_scores_gemma":[0.0000045362144,0.00007502288,0.99233866,0.0000070578867,0.000012640759,0.0014885552,0.00020035927,0.0008162699,0.0026169233,0.00013536212,0.0022955588,0.000009002732],"about_ca_topic_score_codex":0.0044893585,"about_ca_topic_score_gemma":0.0043557016,"teacher_disagreement_score":0.0044893585,"about_ca_system_score_codex":0.0003595918,"about_ca_system_score_gemma":0.00013712118,"threshold_uncertainty_score":0.008926451},"labels":[],"label_agreement":null},{"id":"W4409129455","doi":"10.3847/1538-4357/adbbb7","title":"Infant Type Ia Supernovae from the KMTNet. I. Multicolor Evolution and Populations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Physics; Supernova; Astrophysics; Stellar evolution; Astronomy; Type (biology); Stars; Biology","score_opus":0.01406910389642838,"score_gpt":0.26191398264367166,"score_spread":0.24784487874724329,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409129455","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998331,0.0001728475,0.00030799062,0.000004630123,0.0000016806738,0.000009908106,0.00044447317,0.000011411884,0.00071608974],"genre_scores_gemma":[0.9977557,0.00008782962,0.0005112809,0.000012844066,0.0000031928384,0.000007670655,0.001250828,0.000012851786,0.00035781143],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99959594,0.000055952263,0.00004204594,0.0001636334,0.000078120946,0.00006423119],"domain_scores_gemma":[0.9989704,0.00012931852,0.00048176316,0.00015818936,0.00013066159,0.00012981302],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00041610084,0.00028283274,0.00023735268,0.0018007049,0.00037454916,0.00056329806,0.00033560887,0.0001335119,0.0012300911],"category_scores_gemma":[0.0010016083,0.00014452725,0.00037407508,0.0007332094,0.00023186542,0.0002654881,0.00058706687,0.00022346024,0.0003528728],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000085629894,0.000012758384,0.9870324,0.00000952987,0.000052115378,0.00011778962,0.000050572253,0.00011160076,0.006252101,0.000048901307,0.00005073553,0.0061758067],"study_design_scores_gemma":[0.0000013544342,0.00002340774,0.99808145,0.000003303834,0.000019526067,0.0004689354,0.000036206446,0.00015660672,0.0008694095,0.000043472523,0.00029349283,0.0000028384002],"about_ca_topic_score_codex":0.0019356075,"about_ca_topic_score_gemma":0.0047084666,"teacher_disagreement_score":0.0019356075,"about_ca_system_score_codex":0.0002768639,"about_ca_system_score_gemma":0.00016393204,"threshold_uncertainty_score":0.004115045},"labels":[],"label_agreement":null},{"id":"W4409175648","doi":"10.3847/1538-4357/adb4f3","title":"Deep in the Fields of the Andromeda Halo: Discovery of the Pegasus VII Dwarf Galaxy in UNIONS","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; University of Waterloo; Herzberg Institute of Astrophysics; University of Victoria","funders":"National Astronomical Observatory of Japan; Centre National de la Recherche Scientifique; Canadian Space Agency; Nuclear Safety and Security Commission; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Andromeda; Andromeda Galaxy; Astronomy; Halo; Dwarf galaxy; Astrophysics; Galaxy; Dwarf spheroidal galaxy; Milky Way; Interacting galaxy","score_opus":0.0070375870469188955,"score_gpt":0.22303542214815003,"score_spread":0.21599783510123113,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409175648","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99631506,0.00033349605,0.0002135024,0.00006553419,0.000003477928,0.0000045413713,0.00016708908,0.000016302378,0.002881178],"genre_scores_gemma":[0.9990988,0.00014781683,0.00016288456,0.000024995812,0.0000069746557,0.0000018475112,0.00017428893,0.000004663408,0.00037767092],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999212,0.0000092997025,0.0000023466825,0.000021044847,0.000019784402,0.000026303274],"domain_scores_gemma":[0.9998486,0.000015676651,0.000041075,0.00001787058,0.000009921351,0.00006678414],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000118847,0.00016907348,0.00013717951,0.00079542707,0.00064198975,0.0006101421,0.00019027322,0.00015910735,0.0016315457],"category_scores_gemma":[0.00028917714,0.00008217948,0.00011768128,0.0004918318,0.0005171115,0.0003199244,0.000988498,0.00020889782,0.0003322338],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000272492,0.00007207999,0.9012793,0.000053609652,0.000080455975,0.0019948096,0.003691396,0.00027640173,0.03166128,0.0037602144,0.0015181283,0.0553399],"study_design_scores_gemma":[0.0000057933353,0.00004415459,0.98777986,0.000015600233,0.000016300488,0.0009395032,0.0012849816,0.00015700838,0.0009409746,0.00066020654,0.008149113,0.0000064651767],"about_ca_topic_score_codex":0.0070180097,"about_ca_topic_score_gemma":0.0077615944,"teacher_disagreement_score":0.0070180097,"about_ca_system_score_codex":0.00042395951,"about_ca_system_score_gemma":0.00017216807,"threshold_uncertainty_score":0.013954282},"labels":[],"label_agreement":null},{"id":"W4409205914","doi":"10.3847/1538-4357/adbd40","title":"Polycyclic Aromatic Hydrocarbon and CO(2–1) Emission at 50–150 pc Scales in 70 Nearby Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Agencia Nacional de Investigación y Desarrollo; Agence Nationale de la Recherche; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Physics; Polycyclic aromatic hydrocarbon; Galaxy; Astrophysics; Astronomy; Hydrocarbon; Luminous infrared galaxy; Astrobiology; Organic chemistry","score_opus":0.006715106963981747,"score_gpt":0.2428011440306603,"score_spread":0.23608603706667855,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409205914","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99965227,0.000027394357,0.00004175906,0.0000032792648,3.2662072e-7,0.0000024332176,0.00013243263,0.000006502773,0.00013363281],"genre_scores_gemma":[0.99879444,0.000031640837,0.00018658403,0.000009623625,0.0000028740387,0.0000044178823,0.00085706083,0.000003804481,0.00010952591],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979466,0.000018112598,0.000009925264,0.00007993559,0.000042038737,0.000055343266],"domain_scores_gemma":[0.9994929,0.00009183851,0.00012851892,0.000060845632,0.00005900736,0.00016686012],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001882711,0.00017185905,0.0002321304,0.0011403211,0.00033768086,0.00040613304,0.00034075227,0.00027833384,0.00067560136],"category_scores_gemma":[0.00049903936,0.00025678723,0.00024229636,0.0007968636,0.00037205094,0.00029609937,0.00059135177,0.00016525252,0.00028438368],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011351235,0.0000728366,0.9756752,0.000013893845,0.00008311793,0.000086158296,0.00036476276,0.0004050999,0.017180463,0.000070285554,0.00017508987,0.0057596047],"study_design_scores_gemma":[0.0000015413373,0.000015972952,0.99928516,5.544281e-7,0.0000059950403,0.00002394899,0.000046164427,0.00023802681,0.00028828232,0.000008786586,0.000083943756,0.0000015388609],"about_ca_topic_score_codex":0.024639862,"about_ca_topic_score_gemma":0.040069204,"teacher_disagreement_score":0.024639862,"about_ca_system_score_codex":0.00044195782,"about_ca_system_score_gemma":0.00013021943,"threshold_uncertainty_score":0.04899293},"labels":[],"label_agreement":null},{"id":"W4409206229","doi":"10.3847/1538-4357/adb834","title":"A 100 Mpc<sup>2</sup> Structure Traced by Hyperluminous Galaxies around a Massive <i>z</i> = 2.85 Protocluster","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Dalhousie University; Herzberg Institute of Astrophysics; University of British Columbia","funders":"National Institutes of Natural Sciences; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; National Astronomical Observatory of Japan; National Science Foundation; Korea Astronomy and Space Science Institute; National Radio Astronomy Observatory","keywords":"Physics; Galaxy; Astrophysics; Astronomy","score_opus":0.004746907016037455,"score_gpt":0.2095708306549431,"score_spread":0.20482392363890567,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409206229","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99888355,0.000025891733,0.00019974343,0.000015825142,0.0000013606568,0.0000023405391,0.00013351935,0.000031190226,0.0007066381],"genre_scores_gemma":[0.99936074,0.000009176382,0.00027096015,0.0000071496,0.0000028481052,0.0000014111491,0.00019865543,0.0000028238073,0.00014614458],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999765,0.0000015775448,7.8343277e-7,0.0000066627995,0.000006346384,0.000008126459],"domain_scores_gemma":[0.9998293,0.000014385782,0.000074852105,0.000013398312,0.000017439166,0.00005062318],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000049822556,0.00010704138,0.000092391696,0.00046805877,0.00024253859,0.00024866287,0.0002632722,0.00011772517,0.0012373698],"category_scores_gemma":[0.00013745499,0.00011198747,0.00009197346,0.00030398896,0.00018986453,0.00011686272,0.00030863954,0.00012645613,0.00022153063],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002712576,0.000058054644,0.85747445,0.000028199694,0.00006178724,0.0012521175,0.0004262791,0.0018717184,0.12479238,0.00097490265,0.0013689803,0.011419799],"study_design_scores_gemma":[0.000004723714,0.000028816437,0.9957419,0.000002480757,0.000013203989,0.00021214773,0.00006966967,0.001181985,0.0020980507,0.000108353524,0.0005359872,0.0000026389348],"about_ca_topic_score_codex":0.0039835903,"about_ca_topic_score_gemma":0.00680301,"teacher_disagreement_score":0.0039835903,"about_ca_system_score_codex":0.00023029452,"about_ca_system_score_gemma":0.00007617087,"threshold_uncertainty_score":0.007920802},"labels":[],"label_agreement":null},{"id":"W4409275153","doi":"10.3847/1538-4357/adc07d","title":"Constraints on the X-Ray and Very-high-energy Gamma-Ray Flux from Supernova Remnant W44","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Natural Sciences and Engineering Research Council of Canada; National Energy Research Scientific Computing Center; U.S. Department of Energy; Office of Science; Smithsonian Institution; National Science Foundation","keywords":"Physics; Supernova remnant; Astrophysics; Gamma ray; X-ray; Flux (metallurgy); Supernova; Pulsar; Near-Earth supernova; Astronomy; Neutron star; Nuclear physics","score_opus":0.007341118532191367,"score_gpt":0.2057463524781346,"score_spread":0.19840523394594325,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409275153","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99808806,0.00014480272,0.00042342464,0.000017250568,0.0000027612678,0.0000021768,0.000117828575,0.000016570511,0.001187084],"genre_scores_gemma":[0.9989819,0.000093299066,0.0003291907,0.000016774711,0.000005702085,0.0000034290433,0.00033515974,0.0000064616543,0.00022805373],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997919,0.000027631195,0.000032177795,0.000044276683,0.000056796354,0.000047187918],"domain_scores_gemma":[0.9989084,0.00021723816,0.00041113762,0.00014375473,0.00014942398,0.00016994949],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005757018,0.0003757607,0.00025814766,0.00119561,0.00040945972,0.001032804,0.00042019552,0.00048483495,0.002108327],"category_scores_gemma":[0.001297054,0.00024848606,0.00037514218,0.00033025598,0.00042679516,0.000536599,0.00090902526,0.0002378556,0.00060573267],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029805038,0.000090832815,0.880607,0.00009884635,0.0001590671,0.0006730737,0.0002269005,0.0005884672,0.10662419,0.0016333082,0.00033732457,0.008662981],"study_design_scores_gemma":[0.000014440024,0.00013849256,0.97698337,0.000030060426,0.000060210223,0.0008713521,0.0001248549,0.0015706551,0.017658113,0.00077189464,0.0017580189,0.000018497063],"about_ca_topic_score_codex":0.0011038781,"about_ca_topic_score_gemma":0.0013802273,"teacher_disagreement_score":0.002108327,"about_ca_system_score_codex":0.00019935337,"about_ca_system_score_gemma":0.00010551758,"threshold_uncertainty_score":0.007053077},"labels":[],"label_agreement":null},{"id":"W4409275737","doi":"10.3847/1538-4357/adbbe2","title":"X-Ray Polarization of the High-synchrotron-peak BL Lacertae Object 1ES 1959+650 during Intermediate and High X-Ray Flux States","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Smithsonian Astrophysical Observatory; Instituto de Astrofísica de Andalucía; Istituto Nazionale di Fisica Nucleare; Stockholms Universitet; Aarhus Universitet; Turun Yliopisto; Marshall Space Flight Center; Nuclear Safety and Security Commission; Háskóli Íslands; Istituto Nazionale di Astrofisica; European Commission; Ministerio de Ciencia e Innovación; Goddard Space Flight Center; Universitetet i Oslo; Agencia Estatal de Investigación; Oak Ridge Associated Universities; University of Crete; National Science Foundation; Agenzia Spaziale Italiana; Academy of Finland; Academia Sinica; California Institute of Technology; National Aeronautics and Space Administration; Smithsonian Institution","keywords":"Physics; BL Lac object; X-ray; Synchrotron; Astrophysics; Flux (metallurgy); Polarization (electrochemistry); Astronomy; Synchrotron radiation; High energy; Blazar; Atomic physics; Gamma ray; Optics","score_opus":0.0028015340814435317,"score_gpt":0.19571023023584863,"score_spread":0.1929086961544051,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409275737","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988549,0.000077968536,0.00012730848,0.000012830203,0.0000021256449,0.0000034565398,0.00013602778,0.000015459436,0.0007699153],"genre_scores_gemma":[0.99935395,0.00003315195,0.00008814145,0.000011246236,0.0000062360987,0.0000028221325,0.00030696104,0.000003634838,0.00019384509],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999275,0.0000069020116,0.000003938112,0.000024359812,0.000017352286,0.00001984619],"domain_scores_gemma":[0.9998572,0.000015917296,0.000055146724,0.000014963915,0.000018785322,0.00003785544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022210527,0.0002867081,0.00019579862,0.0008130125,0.00029931942,0.00063677446,0.00019737481,0.00025356436,0.0007261093],"category_scores_gemma":[0.00025807752,0.00018666753,0.00018181397,0.00039190968,0.000250802,0.00023720879,0.00038786785,0.00021017827,0.00022464884],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00067526,0.00010426567,0.7863441,0.000059060585,0.00016242336,0.0009441951,0.0006033491,0.001709027,0.19898218,0.00023832351,0.0003648493,0.009813017],"study_design_scores_gemma":[0.0000054044654,0.000028194549,0.9980844,0.0000028990266,0.000009232844,0.0000615448,0.000057767877,0.00028667093,0.0012128846,0.000015819887,0.00023171942,0.0000033950284],"about_ca_topic_score_codex":0.004195009,"about_ca_topic_score_gemma":0.006621506,"teacher_disagreement_score":0.004195009,"about_ca_system_score_codex":0.00042561855,"about_ca_system_score_gemma":0.00009606778,"threshold_uncertainty_score":0.008341193},"labels":[],"label_agreement":null},{"id":"W4409375189","doi":"10.3847/1538-4357/adbbee","title":"Multiwavelength Study of a Hyperluminous X-Ray Source near NGC 6099: A Strong IMBH Candidate","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Astrophysics; X-ray; Astronomy; Optics","score_opus":0.010010037708415824,"score_gpt":0.24391215914941178,"score_spread":0.23390212144099595,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409375189","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99832827,0.000112239584,0.00031714942,0.000040481616,0.0000032356475,0.00000429063,0.00009574531,0.000014194725,0.0010843597],"genre_scores_gemma":[0.99934834,0.000022772556,0.00027803995,0.000015737605,0.000007080302,0.0000015269618,0.00012518173,0.000003170184,0.0001980841],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999335,0.000004962921,0.0000046652485,0.000023586219,0.00001568169,0.000017586763],"domain_scores_gemma":[0.9997259,0.000032333013,0.000086870845,0.00004375157,0.00003080786,0.00008023229],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016441339,0.00024978872,0.000277082,0.0009462373,0.00062641833,0.0005803896,0.0003188836,0.0003399748,0.0013183232],"category_scores_gemma":[0.00021131037,0.00015196245,0.00020803936,0.00053552043,0.00022541075,0.0002675703,0.00061277096,0.00023623106,0.0003962848],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002891911,0.00012512013,0.8276123,0.000046380886,0.000080232516,0.008719197,0.00058049173,0.00042974702,0.15019353,0.00055230333,0.00037268785,0.010998771],"study_design_scores_gemma":[0.000009018596,0.00009489789,0.98763883,0.000014092779,0.000029837602,0.0031776675,0.00033169746,0.0009396746,0.006097689,0.00025575556,0.0014016648,0.000009343264],"about_ca_topic_score_codex":0.0011036457,"about_ca_topic_score_gemma":0.001609001,"teacher_disagreement_score":0.0013183232,"about_ca_system_score_codex":0.00019686509,"about_ca_system_score_gemma":0.00005921701,"threshold_uncertainty_score":0.004410267},"labels":[],"label_agreement":null},{"id":"W4409407099","doi":"10.3847/1538-4357/adb968","title":"EPOCHS. XI. The Structure and Morphology of Galaxies in the Epoch of Reionization to <i>z</i> ∼ 12.5","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Facilities Council; Space Telescope Science Institute; Nuclear Safety and Security Commission; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Goddard Space Flight Center; University of Manchester; National Aeronautics and Space Administration","keywords":"Reionization; Physics; Epoch (astronomy); Galaxy; Astrophysics; Astronomy; Morphology (biology); Intergalactic medium; Redshift","score_opus":0.004543512919868703,"score_gpt":0.21128862631136472,"score_spread":0.206745113391496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409407099","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96999335,0.00024118766,0.0006356807,0.00009116919,0.000014328906,0.000029761735,0.018366743,0.0006472183,0.009980596],"genre_scores_gemma":[0.9694677,0.00010481204,0.0012275331,0.00003371844,0.000018498802,0.000019549772,0.023200942,0.00014498434,0.0057822675],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993074,0.0000023220118,0.0000038448443,0.000017963263,0.000012746317,0.00003244111],"domain_scores_gemma":[0.9995173,0.00003555991,0.0001944521,0.000055014953,0.00006633956,0.00013133069],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011654101,0.00020892452,0.00015303821,0.0013895484,0.00025059428,0.00056021614,0.00021449062,0.0001557358,0.00459483],"category_scores_gemma":[0.00040966977,0.000103492195,0.00033976874,0.00066868035,0.00012123063,0.00021458512,0.0002593335,0.00021380029,0.0021206995],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004438304,0.000050562987,0.9161786,0.00009237957,0.00007436554,0.00024124276,0.0005717011,0.001223719,0.030483516,0.001158164,0.010294841,0.039187126],"study_design_scores_gemma":[0.0000017939815,0.000012440295,0.99723756,0.0000028106983,0.000005289995,0.000051680614,0.000027006532,0.00025321066,0.0007142363,0.000037077294,0.0016549528,0.0000018596603],"about_ca_topic_score_codex":0.0052546924,"about_ca_topic_score_gemma":0.0054560034,"teacher_disagreement_score":0.0052546924,"about_ca_system_score_codex":0.00020601193,"about_ca_system_score_gemma":0.00008030658,"threshold_uncertainty_score":0.015371263},"labels":[],"label_agreement":null},{"id":"W4409463523","doi":"10.3847/1538-4357/adbb5e","title":"The Merging Galaxy Cluster Environment Affects the Morphology of Radio Active Galactic Nuclei","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Alfred P. Sloan Foundation; National Science Foundation","keywords":"Physics; Active galactic nucleus; Galaxy cluster; Astrophysics; Cluster (spacecraft); Astronomy; Brightest cluster galaxy; Galaxy; Morphology (biology); Radio galaxy","score_opus":0.004262171094636871,"score_gpt":0.20329193996231062,"score_spread":0.19902976886767376,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409463523","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963915,0.000044122018,0.000032004784,0.0000046203795,6.2602174e-7,0.0000010497769,0.000035719586,0.000002238964,0.00024047881],"genre_scores_gemma":[0.9998418,0.000012515368,0.000024510071,0.000002955891,0.000001529185,4.399498e-7,0.00005521576,0.0000013597534,0.000059568083],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99974805,0.000057914956,0.000018728644,0.00005569861,0.000058010475,0.00006162487],"domain_scores_gemma":[0.99862254,0.00019941888,0.00068710576,0.00009103458,0.00013968654,0.0002603059],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026725978,0.0001517435,0.00021655975,0.0008371606,0.00039921404,0.0006741446,0.00024291279,0.00015371387,0.0016083784],"category_scores_gemma":[0.0012451463,0.000098188684,0.00014678412,0.00067022885,0.0004999738,0.00028271734,0.00060717715,0.00011626186,0.00018429891],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000078741505,0.0000087323515,0.9945616,0.0000047483854,0.000031386662,0.000054597764,0.00015194435,0.00010646028,0.0036079558,0.000029224802,0.00003290797,0.0013315965],"study_design_scores_gemma":[3.9254982e-7,0.000011217626,0.99966764,4.552993e-7,0.0000047645685,0.000032372503,0.0001023985,0.000032240147,0.00011074241,0.0000045859006,0.000032473334,7.544245e-7],"about_ca_topic_score_codex":0.0050536264,"about_ca_topic_score_gemma":0.006520707,"teacher_disagreement_score":0.0050536264,"about_ca_system_score_codex":0.00026596896,"about_ca_system_score_gemma":0.00012015744,"threshold_uncertainty_score":0.010048449},"labels":[],"label_agreement":null},{"id":"W4409464387","doi":"10.3847/1538-4357/adbb69","title":"Tracing the Earliest Stages of Star and Cluster Formation in 19 Nearby Galaxies with PHANGS-JWST and HST: Compact 3.3 <i>μ</i>m Polycyclic Aromatic Hydrocarbon Emitters and Their Relation to the Optical Census of Star Clusters","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Space Telescope Science Institute","keywords":"Physics; Star formation; Polycyclic aromatic hydrocarbon; Galaxy; Globular cluster; Astrophysics; Astronomy; Tracing; Star cluster; Astrobiology","score_opus":0.007557625531279922,"score_gpt":0.2228939932342217,"score_spread":0.2153363677029418,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409464387","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995409,0.000021916994,0.00008561249,0.0000035334374,4.1653624e-7,0.0000032724922,0.00015539661,0.0000057543953,0.00018331215],"genre_scores_gemma":[0.99921644,0.000018957606,0.00018363752,0.000004178592,0.0000025491408,0.0000028863165,0.0004623075,0.0000028155239,0.00010622632],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998878,0.0000091563015,0.000007281434,0.00003783617,0.00002701225,0.000030824784],"domain_scores_gemma":[0.99917835,0.000079414756,0.00032097587,0.00007345414,0.00009063596,0.00025707297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019729823,0.00011703557,0.00015031036,0.0012196957,0.00024861642,0.00043796896,0.00021199831,0.00014996062,0.0007544819],"category_scores_gemma":[0.0005855288,0.00012264827,0.00015325843,0.0007607214,0.00023798672,0.00023196978,0.0004858449,0.00013232886,0.00020536747],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000039949504,0.000016164044,0.990404,0.0000048767006,0.0000125145225,0.00009070186,0.00019010087,0.00007137367,0.006227288,0.00003723249,0.000076939505,0.0028288474],"study_design_scores_gemma":[7.783879e-7,0.000009215555,0.99945396,7.2490656e-7,0.0000024198353,0.000040519106,0.000043022883,0.00015605122,0.00020863966,0.000006392866,0.00007748537,7.892769e-7],"about_ca_topic_score_codex":0.012669457,"about_ca_topic_score_gemma":0.022412486,"teacher_disagreement_score":0.012669457,"about_ca_system_score_codex":0.00032525437,"about_ca_system_score_gemma":0.00013649344,"threshold_uncertainty_score":0.025191426},"labels":[],"label_agreement":null},{"id":"W4409464552","doi":"10.3847/1538-4357/adbf12","title":"An Equilibrium Model of the Galaxy Determined by Element Abundance Gradients","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; Flatiron Health; European Space Agency","keywords":"Physics; Abundance (ecology); Astrophysics; Galaxy; Abundance of the chemical elements; Galaxy formation and evolution; Astronomy","score_opus":0.009209010852401256,"score_gpt":0.23646578130944548,"score_spread":0.22725677045704423,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409464552","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.7787352,0.00036418939,0.1971214,0.00094988354,0.000050481038,0.000057119818,0.00062796165,0.00031699162,0.021776779],"genre_scores_gemma":[0.9816922,0.00015183384,0.008757891,0.00009745709,0.000030292375,0.000061955594,0.00018560787,0.00006100442,0.008961684],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999838,0.000039954335,0.0000057396774,0.00005517849,0.000029829736,0.000031373922],"domain_scores_gemma":[0.99962544,0.00011029339,0.0000722526,0.000034902114,0.00008046643,0.00007672547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038982547,0.0004347604,0.00058262114,0.0008360262,0.00057648815,0.0012360981,0.0016303407,0.0008842393,0.0045095147],"category_scores_gemma":[0.0016504352,0.0005154644,0.00067877787,0.00039610857,0.0011201613,0.0017914737,0.0008066707,0.00044352678,0.0011051764],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018705924,0.00006637973,0.014533603,0.000052861702,0.000081198705,0.00031196247,0.00028790295,0.7441854,0.007884657,0.22427127,0.0012648103,0.006872957],"study_design_scores_gemma":[0.00003375286,0.000028376986,0.002311456,0.0000056018885,0.0000104033525,0.000048345697,0.000030043213,0.9706953,0.00019054869,0.025922483,0.0007064905,0.000017233191],"about_ca_topic_score_codex":0.022704449,"about_ca_topic_score_gemma":0.012671486,"teacher_disagreement_score":0.022704449,"about_ca_system_score_codex":0.0014746155,"about_ca_system_score_gemma":0.00068988366,"threshold_uncertainty_score":0.045144618},"labels":[],"label_agreement":null},{"id":"W4409687499","doi":"10.3847/1538-4357/adc30b","title":"Characterizing Magnetic Properties of Young Protostars in Orion","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Physics; Protostar; Astronomy; Astrophysics; Orion Nebula; Stars; Molecular cloud; Star formation","score_opus":0.010346789322794423,"score_gpt":0.22519204115867725,"score_spread":0.21484525183588282,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409687499","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996766,0.000040823605,0.000047178248,0.0000036590745,8.817562e-7,0.0000015502467,0.000077813755,0.000002314346,0.00014920626],"genre_scores_gemma":[0.99949014,0.000032481938,0.000066252025,0.000006639786,0.0000027392696,0.0000016369223,0.00029855737,0.0000023387151,0.00009909121],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994004,0.0000071559484,0.000004553988,0.000020152747,0.000011726485,0.000016443753],"domain_scores_gemma":[0.99970883,0.000027535887,0.00008036731,0.000016520484,0.000054443328,0.00011233628],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001389983,0.00020237765,0.0002066444,0.00094748096,0.00027665624,0.00043858978,0.00014182106,0.00017161833,0.0005041792],"category_scores_gemma":[0.00044958535,0.00011460461,0.00009568635,0.0004583712,0.0002262285,0.00017486184,0.00032657335,0.00012414898,0.00018666967],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008721961,0.000013680196,0.9834116,0.000007747909,0.000017601824,0.00016867394,0.0002210516,0.00007729124,0.013968007,0.000017835924,0.000046473713,0.0019628224],"study_design_scores_gemma":[0.0000013438545,0.000019513816,0.99925774,0.0000011091045,0.0000028469426,0.00011806817,0.000106297295,0.000078500874,0.0002712854,0.0000105476765,0.00013167677,0.0000010642437],"about_ca_topic_score_codex":0.002904123,"about_ca_topic_score_gemma":0.0032735611,"teacher_disagreement_score":0.002904123,"about_ca_system_score_codex":0.00019749586,"about_ca_system_score_gemma":0.00009060761,"threshold_uncertainty_score":0.0057744384},"labels":[],"label_agreement":null},{"id":"W4409687916","doi":"10.3847/1538-4357/adc102","title":"Velocity Structure Correlations between the Nebular, Molecular, and Atmospheric Gases in the Cores of Four Cool Core Clusters","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; University of California, San Diego; National Aeronautics and Space Administration; California Institute of Technology; W. M. Keck Foundation","keywords":"Physics; Astrophysics; Core (optical fiber); Molecular cloud; Astronomy; Astrobiology; Stars","score_opus":0.009430722647510232,"score_gpt":0.22801849664793183,"score_spread":0.2185877740004216,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409687916","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9998286,0.000016607675,0.000022396396,0.0000017046722,2.793365e-7,6.762306e-7,0.000052038482,0.0000020785596,0.000075531556],"genre_scores_gemma":[0.9996573,0.000009111564,0.000049625745,0.0000015175285,9.235861e-7,0.0000011233637,0.00021558705,0.0000012483611,0.00006353934],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991536,0.0000067789624,0.000005105009,0.000030349347,0.000017069246,0.000025374617],"domain_scores_gemma":[0.999627,0.000044822962,0.00011368217,0.000030031619,0.00006807514,0.00011639726],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016607695,0.00015330549,0.00016173522,0.000999286,0.00027166776,0.00034499212,0.00022285896,0.00013495506,0.00058508693],"category_scores_gemma":[0.000495552,0.00011234245,0.00015230509,0.00045932605,0.00020146293,0.00015971504,0.0003617383,0.00007931982,0.000111548376],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000079216225,0.000013935356,0.9898245,0.000005697159,0.00002938392,0.000026798236,0.0003253588,0.00035078614,0.007538298,0.00009851589,0.00008739151,0.0016201829],"study_design_scores_gemma":[0.000001139828,0.000009232841,0.9993862,7.5004823e-7,0.0000028331858,0.00001058621,0.000057540565,0.00030275877,0.00015991037,0.0000075858675,0.000060363673,9.953957e-7],"about_ca_topic_score_codex":0.025849361,"about_ca_topic_score_gemma":0.029913517,"teacher_disagreement_score":0.025849361,"about_ca_system_score_codex":0.00033374203,"about_ca_system_score_gemma":0.00014029913,"threshold_uncertainty_score":0.0513978},"labels":[],"label_agreement":null},{"id":"W4409824981","doi":"10.3847/1538-4357/adc449","title":"The Impact of the Galactic Bar and the Large Magellanic Cloud on Hypervelocity Star Trajectories","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McMaster University","funders":"","keywords":"Physics; Hypervelocity; Large Magellanic Cloud; Astronomy; Milky Way; Astrophysics; Bar (unit); Star (game theory); Galaxy","score_opus":0.006773032741744206,"score_gpt":0.23650868534140396,"score_spread":0.22973565259965975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409824981","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99862385,0.00004820677,0.00048218152,0.000047648915,0.000006931048,0.0000047088283,0.00012766599,0.000020996265,0.00063781574],"genre_scores_gemma":[0.9994899,0.000020525345,0.00022394372,0.000010008197,0.000002041533,0.0000024545845,0.0001224103,0.000011175806,0.00011742997],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99985826,0.000044572338,0.000007572569,0.000023905774,0.000021228583,0.00004438773],"domain_scores_gemma":[0.99908125,0.0004045555,0.00014480062,0.00008754364,0.000117641284,0.00016418908],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006658803,0.00038231906,0.0003350146,0.00043042947,0.00053173536,0.00099903,0.0006479303,0.00065812137,0.0013324776],"category_scores_gemma":[0.0027345277,0.000228935,0.0006631697,0.00033842228,0.00047874197,0.00066202006,0.0005692792,0.0004639618,0.00018108886],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017089958,0.00009341057,0.17042996,0.000032033728,0.0001304944,0.00022211314,0.00007968622,0.8215187,0.0029809354,0.00092747796,0.0003757015,0.0030386117],"study_design_scores_gemma":[0.000074807314,0.0002289737,0.0638309,0.000019982117,0.000054661974,0.00008421649,0.00017663502,0.93250376,0.002009717,0.00039012564,0.0006021548,0.000024070257],"about_ca_topic_score_codex":0.023615733,"about_ca_topic_score_gemma":0.016957896,"teacher_disagreement_score":0.023615733,"about_ca_system_score_codex":0.00078148633,"about_ca_system_score_gemma":0.00060676696,"threshold_uncertainty_score":0.04695654},"labels":[],"label_agreement":null},{"id":"W4409956049","doi":"10.3847/1538-4357/adc4db","title":"Using Two-frequency Dust Spectral Matching to Separate Galactic Synchrotron and Free–Free Temperature Foregrounds from the Cosmic Microwave Background","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Physics; Cosmic microwave background; Synchrotron; Astrophysics; Microwave; Astronomy; COSMIC cancer database; Cosmic dust; Cosmic infrared background; Optics","score_opus":0.01331257488735806,"score_gpt":0.25991017917645926,"score_spread":0.24659760428910119,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409956049","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6017964,0.00010424677,0.39307308,0.000058688438,0.00003734272,0.000033324224,0.0005486513,0.001349424,0.002998866],"genre_scores_gemma":[0.7956386,0.0000552552,0.20191577,0.000027723343,0.000031515487,0.000026692773,0.0012423502,0.00020466362,0.0008574526],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99984694,0.000020153751,0.000008075748,0.0000481203,0.000047239413,0.000029475921],"domain_scores_gemma":[0.99971753,0.00005159524,0.000050836574,0.00008149617,0.000079009675,0.000019421554],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027490561,0.000299051,0.0002572386,0.0015019102,0.0002438547,0.0006488177,0.0003941857,0.00024443804,0.001366844],"category_scores_gemma":[0.0008716866,0.0001896626,0.00046009864,0.0009476091,0.00019105895,0.00040282187,0.00048207393,0.0002399146,0.00043027912],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011814976,0.00034792477,0.07318485,0.00014682165,0.00039842667,0.00019684201,0.00025616813,0.050902307,0.39027643,0.004885081,0.0014397945,0.47678387],"study_design_scores_gemma":[0.00013665033,0.00015016636,0.17290568,0.00001677421,0.00022905313,0.00034118677,0.00017168256,0.6421603,0.16755037,0.006929922,0.009328275,0.00007995746],"about_ca_topic_score_codex":0.0020274837,"about_ca_topic_score_gemma":0.003055897,"teacher_disagreement_score":0.0020274837,"about_ca_system_score_codex":0.00025693586,"about_ca_system_score_gemma":0.00028330125,"threshold_uncertainty_score":0.0045725703},"labels":[],"label_agreement":null},{"id":"W4409957579","doi":"10.3847/1538-4357/adc719","title":"Dynamics of Star Cluster Formation: The Effects of Ongoing Star Formation and Stellar Feedback","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Astrophysics; Star cluster; Star (game theory); Star formation; Astronomy; Cluster (spacecraft); Stellar evolution; Stellar dynamics; Dynamics (music); Stars; Blue straggler; Stellar physics","score_opus":0.004503147036499517,"score_gpt":0.206129341008781,"score_spread":0.2016261939722815,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4409957579","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99441093,0.000045378325,0.0012715863,0.00017829695,0.00002480762,0.000030307978,0.00019225654,0.000114722185,0.0037317444],"genre_scores_gemma":[0.99825484,0.000026463882,0.0010036906,0.000047069294,0.00000687255,0.000012932422,0.00016123163,0.00003595362,0.0004509433],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997948,0.00004284761,0.0000073434953,0.000031335727,0.00004797396,0.00007567724],"domain_scores_gemma":[0.9992467,0.00025324963,0.00009382327,0.000055747925,0.000105705854,0.0002448111],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049010303,0.0005123228,0.00069090124,0.00043699524,0.0010860219,0.001204832,0.0013382789,0.0011153633,0.0022402785],"category_scores_gemma":[0.0020650937,0.00043618216,0.0006045071,0.00052074157,0.0013815956,0.0007185295,0.0008962089,0.0011797493,0.00016830703],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023969244,0.00027253234,0.012544165,0.000027114991,0.00007413841,0.00024095479,0.00012106474,0.97905755,0.0043391576,0.0015142137,0.00045968505,0.001109801],"study_design_scores_gemma":[0.00012225853,0.000111298235,0.0047970917,0.000005632485,0.00001689226,0.000023028575,0.000069591886,0.9931004,0.0011611143,0.0002986223,0.0002768508,0.000017250879],"about_ca_topic_score_codex":0.05123793,"about_ca_topic_score_gemma":0.026812715,"teacher_disagreement_score":0.05123793,"about_ca_system_score_codex":0.0020389364,"about_ca_system_score_gemma":0.0016112338,"threshold_uncertainty_score":0.10187942},"labels":[],"label_agreement":null},{"id":"W4410034591","doi":"10.3847/1538-4357/adc38d","title":"Jet-mode Feedback in NGC 5972: Insights from Resolved MUSE, GMRT, and VLA Observations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Physics; Astrophysics; Jet (fluid); Giant Metrewave Radio Telescope; Astronomy; Mode (computer interface); Radio galaxy; Galaxy","score_opus":0.015444612558689523,"score_gpt":0.24144242596840512,"score_spread":0.2259978134097156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410034591","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983341,0.00020637702,0.00022949564,0.000024961393,0.0000044687076,0.0000044729545,0.00034754473,0.000054164455,0.00079431426],"genre_scores_gemma":[0.9989973,0.000046186702,0.00031897315,0.000011949265,0.000009496722,0.0000035534545,0.00048669937,0.00001298235,0.00011292915],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998479,0.00000990444,0.000006505962,0.00004951866,0.0000412665,0.000044851895],"domain_scores_gemma":[0.99969053,0.000030084297,0.000101375634,0.000032623415,0.00003891853,0.00010645393],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000228057,0.00033783916,0.00048327266,0.001717177,0.0004899496,0.0006054072,0.00043799297,0.00034529154,0.001034115],"category_scores_gemma":[0.0005599353,0.00020229003,0.00030011352,0.00093848875,0.00029405358,0.00032336373,0.0006286519,0.00022298051,0.00026985246],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029555766,0.00009647111,0.81708235,0.00009253722,0.00012793284,0.0021574365,0.00087302754,0.0017879587,0.15628225,0.00030193158,0.0008921575,0.020010347],"study_design_scores_gemma":[0.000009686238,0.000028765548,0.9966517,0.000009628546,0.000036088168,0.00023136649,0.00022065757,0.001236515,0.0008228004,0.000071876064,0.0006679362,0.000012973478],"about_ca_topic_score_codex":0.0150797935,"about_ca_topic_score_gemma":0.02338083,"teacher_disagreement_score":0.0150797935,"about_ca_system_score_codex":0.0004209015,"about_ca_system_score_gemma":0.00013760003,"threshold_uncertainty_score":0.029984057},"labels":[],"label_agreement":null},{"id":"W4410176976","doi":"10.3847/1538-4357/adb979","title":"Chandra Detects Low-luminosity Active Galactic Nucleus with <i>M</i> <sub>BH</sub> = 10<sup>4</sup>–10<sup>6</sup> <i> M</i> <sub>⊙</sub> in Nearby (<i>z</i> &lt; 0.5) Dwarf and Star-forming Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Leibniz-Gemeinschaft; Smithsonian Astrophysical Observatory; University of Colorado Boulder; National Astronomical Observatories, Chinese Academy of Sciences; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; New Mexico State University; Nanjing University; Natural Science Foundation of Shanghai; China National Textile and Apparel Council; National Science Foundation; Yunnan University; Yale University; University of Toronto; Smithsonian Institution; National Natural Science Foundation of China; École Polytechnique Fédérale de Lausanne; Space Telescope Science Institute; Universidad Nacional Autónoma de México; Goddard Space Flight Center; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Harvard University; Ohio State University; Leibniz-Institut für Astrophysik Potsdam; National Aeronautics and Space Administration","keywords":"Physics; Luminosity; Astrophysics; Active galactic nucleus; Astronomy; Nucleus; Galaxy; Medicine","score_opus":0.004823217759519361,"score_gpt":0.1908896448198124,"score_spread":0.18606642706029305,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410176976","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953442,0.00037584748,0.00065808586,0.000025732099,0.0000070192373,0.0000136459885,0.0003766611,0.0001625297,0.0030362678],"genre_scores_gemma":[0.9979691,0.0000715008,0.0012604728,0.000025251333,0.000009133999,0.0000049886453,0.0002600391,0.000008044898,0.0003914587],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998443,0.000016972072,0.000013864294,0.00003377334,0.000043401582,0.000047683407],"domain_scores_gemma":[0.99905664,0.00016113216,0.00029867646,0.00010907687,0.000117291784,0.00025718068],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027291517,0.00022584294,0.00021666942,0.0012042657,0.00026713416,0.0005853081,0.00040869092,0.00018907723,0.0033690662],"category_scores_gemma":[0.0007498901,0.0001677722,0.00016202124,0.0004986374,0.0002805034,0.0003462079,0.00038268242,0.00017842367,0.00052706],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00029591992,0.000069505855,0.9122017,0.000106214975,0.00008238256,0.00072213646,0.00016354427,0.00013927478,0.06466317,0.00034543945,0.00087591977,0.02033479],"study_design_scores_gemma":[0.000008282228,0.000083964675,0.9846095,0.000017358001,0.000036088244,0.0019646257,0.00017125477,0.00044766854,0.011255246,0.00013058144,0.0012676977,0.000007779454],"about_ca_topic_score_codex":0.0011566234,"about_ca_topic_score_gemma":0.0026377297,"teacher_disagreement_score":0.0033690662,"about_ca_system_score_codex":0.00013491196,"about_ca_system_score_gemma":0.000107534186,"threshold_uncertainty_score":0.011270642},"labels":[],"label_agreement":null},{"id":"W4410311698","doi":"10.3847/1538-4357/adbcab","title":"Cloud-scale Gas Properties, Depletion Times, and Star Formation Efficiency per Freefall Time in PHANGS–ALMA","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":15,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Radio Astronomy Observatory","keywords":"Physics; Astrophysics; Cloud computing; Scale (ratio); Star formation; Astronomy; Star (game theory); Molecular cloud; Stars","score_opus":0.006377027864741334,"score_gpt":0.20775351273087056,"score_spread":0.20137648486612922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410311698","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9983303,0.000028885808,0.00020101384,0.000019481766,0.0000029038922,0.000004212593,0.000623298,0.000030791976,0.00075920054],"genre_scores_gemma":[0.9981988,0.000012757314,0.00020638782,0.000019266588,0.000006491219,0.000005523456,0.0011287521,0.00001224277,0.00040986307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998621,0.000014536302,0.0000077873365,0.000046192217,0.000028496279,0.000040897667],"domain_scores_gemma":[0.9989416,0.00014327896,0.000321407,0.00015939519,0.00015815959,0.0002761835],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002874964,0.0001464743,0.00021261594,0.0009729689,0.00030041265,0.0006204625,0.0003370847,0.00016107652,0.0025940593],"category_scores_gemma":[0.0012542837,0.00014194836,0.00028565625,0.00058370194,0.00029883126,0.00055309857,0.00039377954,0.0002075951,0.00039470562],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015216049,0.000034117227,0.98768103,0.000012328062,0.00008484674,0.0001282222,0.0001966866,0.0018089196,0.0039759246,0.00028051075,0.00076199183,0.004883261],"study_design_scores_gemma":[0.000008631161,0.00002240154,0.99417204,0.0000038901576,0.000016186901,0.00005158069,0.00013106871,0.0037876272,0.0007590908,0.00012291342,0.00091807643,0.000006532906],"about_ca_topic_score_codex":0.025202595,"about_ca_topic_score_gemma":0.027382974,"teacher_disagreement_score":0.025202595,"about_ca_system_score_codex":0.0005772177,"about_ca_system_score_gemma":0.00017669426,"threshold_uncertainty_score":0.05011183},"labels":[],"label_agreement":null},{"id":"W4410524747","doi":"10.3847/1538-4357/adc7ff","title":"Discovery of Small-scale Flows in the Void of a Coronal Mass Ejection with High-cadence Images Acquired by the Metis Coronagraph on Board Solar Orbiter","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Bundesministerium für Wirtschaft und Energie; Istituto Nazionale di Astrofisica; Agenzia Spaziale Italiana; Fundación Carmen y Severo Ochoa","keywords":"Orbiter; Coronagraph; Physics; Coronal mass ejection; Astronomy; Cadence; Scale (ratio); Astrophysics; Corona (planetary geology); Solar wind; Astrobiology; Exoplanet; Plasma; Stars; Venus","score_opus":0.004252960901271351,"score_gpt":0.20726793259655946,"score_spread":0.2030149716952881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410524747","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9953435,0.00012736136,0.0006705231,0.000092001195,0.000016335618,0.00001604954,0.00072220864,0.000097984,0.0029138878],"genre_scores_gemma":[0.9970931,0.000033580473,0.0011994133,0.000026314192,0.0000333678,0.0000071375825,0.0010506957,0.000016263904,0.00054010365],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996626,0.0000017930822,0.0000012840637,0.000009782818,0.000008954935,0.000011859922],"domain_scores_gemma":[0.9998223,0.000021477861,0.00004251339,0.000023492146,0.00002364192,0.00006664215],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011288324,0.00011315342,0.00010794957,0.0008667446,0.00027592658,0.0004341106,0.0001883634,0.00027506554,0.0010741169],"category_scores_gemma":[0.00025109196,0.000112257534,0.00013569536,0.00037983767,0.0001375195,0.00020505147,0.0003445686,0.00025051113,0.00016913717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009641288,0.00043761847,0.5559283,0.00011871309,0.00020918716,0.008339742,0.0011806272,0.0017110596,0.36768547,0.0019270479,0.0070035155,0.05449449],"study_design_scores_gemma":[0.000014736719,0.00005156577,0.99054223,0.000008240921,0.000016239497,0.0005514506,0.0001091077,0.0026198088,0.0035979594,0.00009653178,0.0023856487,0.0000066184575],"about_ca_topic_score_codex":0.0021026945,"about_ca_topic_score_gemma":0.003988861,"teacher_disagreement_score":0.0021026945,"about_ca_system_score_codex":0.00016885098,"about_ca_system_score_gemma":0.00009775753,"threshold_uncertainty_score":0.0041808486},"labels":[],"label_agreement":null},{"id":"W4410618258","doi":"10.3847/1538-4357/adc99e","title":"Traversing the Star-forming Main Sequence with Molecular Gas Stacks of <i>z</i> ∼ 1.6 Cluster Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; University of Toronto; York University","funders":"National Radio Astronomy Observatory; Space Telescope Science Institute","keywords":"Physics; Cluster (spacecraft); Astrophysics; Galaxy cluster; Sequence (biology); Astronomy; Galaxy; Traverse; Star (game theory)","score_opus":0.007284388500932216,"score_gpt":0.23137402657856812,"score_spread":0.2240896380776359,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410618258","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987961,0.000056440313,0.00019613504,0.000017172333,0.0000017094366,0.0000024669964,0.000484729,0.000050885326,0.00039447634],"genre_scores_gemma":[0.9977574,0.000035966867,0.00048993184,0.000014846624,0.0000051657057,0.0000027223484,0.0014775802,0.000015417743,0.00020106255],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981195,0.000009573075,0.0000064323817,0.00007650828,0.000026983631,0.00006864296],"domain_scores_gemma":[0.9993807,0.00005623419,0.0002124048,0.00008376441,0.00010474028,0.00016213443],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002164361,0.00023677158,0.000257565,0.0013575036,0.0003998985,0.00082785473,0.00029821164,0.00018117385,0.0016631205],"category_scores_gemma":[0.00067521515,0.00016525158,0.00035292614,0.0009309514,0.00028587665,0.00042924716,0.0006128668,0.00024077256,0.000540096],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013991974,0.000025317,0.97532475,0.000023031569,0.000086685715,0.00006398177,0.00048485232,0.0006007073,0.01296553,0.00024078584,0.00070244604,0.009341994],"study_design_scores_gemma":[0.0000011034006,0.000014636995,0.99813616,0.000003273114,0.000015616642,0.00004014262,0.00016460592,0.00051657774,0.0006042963,0.000063430496,0.00043739463,0.0000028412044],"about_ca_topic_score_codex":0.009759597,"about_ca_topic_score_gemma":0.010600738,"teacher_disagreement_score":0.009759597,"about_ca_system_score_codex":0.00029698937,"about_ca_system_score_gemma":0.00014675417,"threshold_uncertainty_score":0.019405603},"labels":[],"label_agreement":null},{"id":"W4410701749","doi":"10.3847/1538-4357/adcabf","title":"Learning to See: Applying Inverse Recurrent Inference Machines to See through Refractive Scattering","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Optical measurement and interference techniques","field":"Computer Science","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Perimeter Institute; University of Waterloo","funders":"","keywords":"Physics; Inference; Inverse scattering problem; Scattering; Inverse problem; Inverse; Optics; Theoretical physics; Artificial intelligence; Mathematical analysis; Geometry; Computer science","score_opus":0.03283996858878922,"score_gpt":0.317383135273618,"score_spread":0.28454316668482876,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410701749","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.26029253,0.0003528354,0.7341092,0.00080857344,0.000090193855,0.000041732645,0.00011960544,0.001488682,0.0026966012],"genre_scores_gemma":[0.93530226,0.000058074336,0.062578954,0.00013202232,0.00004433671,0.000030699895,0.00015090151,0.000059406415,0.0016433765],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981374,0.00006871579,0.000007244324,0.000046464887,0.0000323115,0.000031503583],"domain_scores_gemma":[0.9983809,0.0011456414,0.00013911532,0.00012019639,0.00015468031,0.000059367023],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008957825,0.00057949737,0.0006840478,0.00028435522,0.00028679447,0.00055580353,0.0012068368,0.00084664754,0.0011420393],"category_scores_gemma":[0.003572177,0.0004183835,0.00049926847,0.00022158344,0.00066661055,0.0007960287,0.00061419443,0.0010000565,0.00019625168],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004586235,0.000037468402,0.0010527723,0.000016151393,0.000028140525,0.000044838034,0.000031075673,0.9743326,0.0011563869,0.002599087,0.0003709411,0.020284748],"study_design_scores_gemma":[0.0000011606229,0.0000029499427,0.000025246072,4.229192e-7,6.532259e-7,9.809711e-7,9.63676e-7,0.9992467,0.0001092411,0.000595885,0.000015181304,6.831994e-7],"about_ca_topic_score_codex":0.008707543,"about_ca_topic_score_gemma":0.008110062,"teacher_disagreement_score":0.008707543,"about_ca_system_score_codex":0.0007318858,"about_ca_system_score_gemma":0.0006123138,"threshold_uncertainty_score":0.017313719},"labels":[],"label_agreement":null},{"id":"W4410758494","doi":"10.3847/1538-4357/adca38","title":"Exploring the Spectral Energy Distributions of Luminous Broad Absorption Line Quasars at High Redshift","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Quasar; Redshift; Astrophysics; Astronomy; Spectral line; Red shift; Spectral energy distribution; Absorption (acoustics); Absorption spectroscopy; Emission spectrum; Line (geometry); Optics; Galaxy","score_opus":0.014979387892181896,"score_gpt":0.21856948247255964,"score_spread":0.20359009458037775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410758494","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992937,0.000037995444,0.0001641382,0.00000718347,3.9945994e-7,9.500985e-7,0.0002308186,0.000009406828,0.00025548923],"genre_scores_gemma":[0.9993155,0.000020077145,0.0001350549,0.0000044504804,0.0000018718248,0.0000011461075,0.00043072383,0.0000026926887,0.000088461],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998902,0.000011400935,0.000006456437,0.000033590448,0.000026929001,0.000031400283],"domain_scores_gemma":[0.9993451,0.00010899948,0.00029048737,0.000058582515,0.000066909844,0.00012989219],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003304815,0.00017145151,0.0001696424,0.0025045422,0.0001906804,0.0005679825,0.0001848845,0.00017766785,0.0013606916],"category_scores_gemma":[0.0005172187,0.0001063687,0.0002090391,0.0011292541,0.0001909484,0.00030989942,0.0004657022,0.00016860741,0.00025625943],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000416578,0.00002066944,0.9869157,0.000005612059,0.000046489393,0.00004123861,0.00013890583,0.00019029355,0.008670735,0.00011037708,0.00008462994,0.003733713],"study_design_scores_gemma":[4.5889584e-7,0.000007524406,0.99947935,7.3138307e-7,0.0000042936645,0.00002352724,0.000053897344,0.00013657691,0.0001930232,0.000022025102,0.000077795135,8.9178695e-7],"about_ca_topic_score_codex":0.0027735087,"about_ca_topic_score_gemma":0.0043626926,"teacher_disagreement_score":0.0027735087,"about_ca_system_score_codex":0.00014332449,"about_ca_system_score_gemma":0.0000474214,"threshold_uncertainty_score":0.005514741},"labels":[],"label_agreement":null},{"id":"W4410790771","doi":"10.3847/1538-4357/adcec5","title":"Spinning Spectral Sirens: Robust Cosmological Measurement Using Mass–Spin Correlations in the Binary Black Hole Population","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Cosmology and Gravitation Theories","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Physics; Astrophysics; Binary number; Black hole (networking); Spin (aerodynamics); Spinning; Population; Astronomy; Binary black hole; Cosmology; Theoretical physics; Gravitational wave; Thermodynamics","score_opus":0.03557773692243526,"score_gpt":0.28414642194687545,"score_spread":0.24856868502444018,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410790771","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8986887,0.00019512807,0.08571438,0.00018602514,0.00003023689,0.000059598395,0.004018415,0.0024565754,0.008650973],"genre_scores_gemma":[0.9821333,0.000027906168,0.016404478,0.000026221993,0.000030679512,0.00001547952,0.0010538574,0.00006539049,0.0002426504],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996363,0.00012088367,0.000018109089,0.000098918164,0.00009400515,0.000031742307],"domain_scores_gemma":[0.9974354,0.00065257377,0.00090948516,0.00054574263,0.00020857163,0.00024830815],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0015159928,0.00024301844,0.00021701449,0.003011636,0.0002785417,0.00086721795,0.0004132791,0.00031253506,0.001459585],"category_scores_gemma":[0.0043751565,0.00022468077,0.00016725852,0.0014920734,0.0002634236,0.00059473095,0.00069602,0.0003240229,0.00047976626],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003979316,0.00017505909,0.7815984,0.000110718385,0.0003533316,0.00034514768,0.00055623637,0.01611032,0.055363864,0.014793179,0.0063243927,0.12387149],"study_design_scores_gemma":[0.000029416442,0.000058502475,0.79713225,0.000019437854,0.000049589456,0.00023293514,0.00010019103,0.17057046,0.020590007,0.0069218497,0.004213002,0.00008236273],"about_ca_topic_score_codex":0.0015336018,"about_ca_topic_score_gemma":0.0027530354,"teacher_disagreement_score":0.003011636,"about_ca_system_score_codex":0.0002810254,"about_ca_system_score_gemma":0.00014760296,"threshold_uncertainty_score":0.00801748},"labels":[],"label_agreement":null},{"id":"W4410791114","doi":"10.3847/1538-4357/adcdff","title":"A Large-scale Search for Photometrically Variable Active Galactic Nuclei in Dwarf Galaxies Using the Young Supernova Experiment","year":2025,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Science and Technology Facilities Council; Office of Science; York University; Space Telescope Science Institute; Villum Fonden; National Centre for Supercomputing Applications; Carnegie Mellon University; College of Engineering, Michigan State University; University of Washington; Alfred P. Sloan Foundation; Princeton University; Johns Hopkins University; Harvard University; University of California, Santa Cruz; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Vanderbilt University; European Commission; U.S. Department of Energy; University of Illinois at Urbana-Champaign; Nuclear Safety and Security Commission; Gordon and Betty Moore Foundation; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Astrophysics; Supernova; Astronomy; Galaxy; Active galactic nucleus","score_opus":0.015393935348626165,"score_gpt":0.2690147388216303,"score_spread":0.25362080347300414,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410791114","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9977373,0.00007386779,0.00044902085,0.00003085606,0.0000035018104,0.000024915944,0.0012162654,0.000026252912,0.00043811052],"genre_scores_gemma":[0.99476045,0.000067802604,0.0011230021,0.000032082036,0.00000993857,0.000022637312,0.0034629772,0.000019450834,0.0005016073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99934334,0.00022568663,0.00004991488,0.00018402464,0.000100709556,0.00009636249],"domain_scores_gemma":[0.99729544,0.00072626525,0.0005797873,0.00045231413,0.00017278302,0.00077348144],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019105852,0.00029998363,0.000366024,0.0017635194,0.0005786229,0.00071982655,0.00033853296,0.00023666683,0.0010188323],"category_scores_gemma":[0.0016380738,0.00019646849,0.00051146874,0.001016582,0.00036352282,0.00034961922,0.0008223895,0.0003283704,0.00037909677],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00014068853,0.000076660675,0.9934482,0.000009330093,0.00014885854,0.00015516941,0.00009385544,0.00028720775,0.0024975399,0.0001391942,0.00041377702,0.0025894863],"study_design_scores_gemma":[0.000013933145,0.00007674654,0.99759406,0.0000022620545,0.000046880585,0.00011254705,0.00016296156,0.0007002609,0.0004695222,0.000059433823,0.000755012,0.000006280029],"about_ca_topic_score_codex":0.010856367,"about_ca_topic_score_gemma":0.021811066,"teacher_disagreement_score":0.010856367,"about_ca_system_score_codex":0.000302402,"about_ca_system_score_gemma":0.0005652194,"threshold_uncertainty_score":0.021586359},"labels":[],"label_agreement":null},{"id":"W4410791141","doi":"10.3847/1538-4357/adce80","title":"The JCMT BISTRO-3 Survey: Variation of Magnetic Field Orientations on Parsec and Subparsec Scales in the Massive Star-forming Region G28.34+0.06","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Centre for Research in Astrophysics of Québec; University of Victoria; Herzberg Institute of Astrophysics","funders":"National Institutes of Natural Sciences; Alliance of International Science Organizations; Quỹ Đổi mới sáng tạo Vingroup; National Astronomical Observatory of Japan; Ministerio de Ciencia e Innovación; National Research Foundation of Korea; Ministry of Education, Science and Technology; Korea Astronomy and Space Science Institute; National Natural Science Foundation of China; Science and Technology Facilities Council; National Research Foundation; Science and Engineering Research Board; Japan Society for the Promotion of Science; Tập đoàn Vingroup - Công ty CP; Ministerio de Ciencia, Innovación y Universidades; Academia Sinica; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Ministry of Science and ICT, South Korea; Arthritis National Research Foundation","keywords":"Physics; Astrophysics; Parsec; Star formation; Astronomy; Variation (astronomy); Magnetic field; Star (game theory); Stars","score_opus":0.013469235336268459,"score_gpt":0.2554418454636443,"score_spread":0.24197261012737584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410791141","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99866545,0.000018574356,0.00003740722,0.000014122542,9.999163e-7,0.0000033689912,0.0008745168,0.000017487224,0.00036816113],"genre_scores_gemma":[0.99688596,0.000022946593,0.00020929177,0.000020569585,0.0000064849446,0.000007168349,0.002642486,0.000009658568,0.00019540406],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.000009789303,0.0000064193937,0.00003864061,0.000030674117,0.000032255404],"domain_scores_gemma":[0.99932885,0.000053635584,0.00024745538,0.00005901648,0.000093881456,0.00021725644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001447221,0.00018553225,0.00020762953,0.0014301729,0.00024753666,0.0003928875,0.00029154707,0.0002223148,0.00097651314],"category_scores_gemma":[0.00052262796,0.00012622638,0.0001578975,0.00082131464,0.0001937042,0.0002116814,0.0005649008,0.00019964993,0.0002593765],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009854647,0.0000321525,0.98111206,0.000013100567,0.00003576606,0.000111564856,0.0002101934,0.00020701873,0.014143723,0.000056849694,0.0005701057,0.003409008],"study_design_scores_gemma":[0.0000027404553,0.0000048385773,0.99953663,7.1209115e-7,0.0000020368948,0.000019288565,0.000025094849,0.00017090394,0.00011428679,0.0000037358193,0.00011880468,9.560473e-7],"about_ca_topic_score_codex":0.015949113,"about_ca_topic_score_gemma":0.032319844,"teacher_disagreement_score":0.015949113,"about_ca_system_score_codex":0.0003412337,"about_ca_system_score_gemma":0.00016070617,"threshold_uncertainty_score":0.031712532},"labels":[],"label_agreement":null},{"id":"W4410836445","doi":"10.3847/1538-4357/adcac4","title":"Unveiling Two Deeply Embedded Young Protostars in the S68N Class 0 Protostellar Core with JWST/NIRSpec","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Protostar; Physics; Core (optical fiber); Astrophysics; Class (philosophy); Astronomy; Star formation; Stars","score_opus":0.010735953603132377,"score_gpt":0.2671594110491007,"score_spread":0.2564234574459683,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410836445","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99943095,0.000020702337,0.0001292447,0.0000065584877,0.0000013864266,0.000001901641,0.00006517801,0.000016974376,0.00032707627],"genre_scores_gemma":[0.9991291,0.00001298051,0.00048931834,0.000009174991,0.0000033059177,0.0000010355773,0.00019673743,0.0000063646703,0.00015197937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999535,0.0000021886544,0.000001418746,0.000012122945,0.0000111032505,0.000019692106],"domain_scores_gemma":[0.9998609,0.000010708148,0.000039220133,0.0000138496835,0.000017940882,0.00005736758],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000088312605,0.00019439175,0.00013273781,0.00068968546,0.00024519197,0.00028176504,0.0001867325,0.00017624834,0.00061538623],"category_scores_gemma":[0.00012649255,0.0001339374,0.00018069286,0.00026990083,0.00013499727,0.00017027245,0.00031946084,0.00013727961,0.000187188],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034224134,0.00014498585,0.67459816,0.000032405773,0.00007987827,0.004061375,0.0005682335,0.0012536853,0.3018813,0.00018242691,0.00054109434,0.016314209],"study_design_scores_gemma":[0.0000062299396,0.00006648476,0.99006116,0.00000441605,0.000015783808,0.0005979479,0.000246768,0.0026812763,0.005580763,0.00004730897,0.00068682706,0.000005131372],"about_ca_topic_score_codex":0.0029461584,"about_ca_topic_score_gemma":0.007692298,"teacher_disagreement_score":0.0029461584,"about_ca_system_score_codex":0.00014703839,"about_ca_system_score_gemma":0.000081090104,"threshold_uncertainty_score":0.0058580637},"labels":[],"label_agreement":null},{"id":"W4410836541","doi":"10.3847/1538-4357/adc995","title":"A Holistic Exploration of the Potentially Recoverable Redshift Information of Stage IV Galaxy Surveys","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Brinson Foundation; Gordon and Betty Moore Foundation; Schmidt Futures","keywords":"Physics; Galaxy; Redshift; Astrophysics; Astronomy; Redshift survey; Galaxy formation and evolution","score_opus":0.021332700277099194,"score_gpt":0.279870730895713,"score_spread":0.2585380306186138,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410836541","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.72353137,0.0017541011,0.2561038,0.0026280773,0.000027810464,0.00011368999,0.0024891284,0.00026693894,0.013085033],"genre_scores_gemma":[0.9741993,0.00035204084,0.024023257,0.0001272033,0.000028807819,0.00003362731,0.00075255183,0.000026904745,0.0004563389],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99480164,0.0025282507,0.00025762786,0.0006614851,0.0014301519,0.0003208901],"domain_scores_gemma":[0.9672349,0.01839524,0.0061897472,0.004661282,0.0027025444,0.0008162297],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.012939759,0.0007793289,0.00086647755,0.0049478146,0.0005322001,0.0037788618,0.0015344314,0.0010595684,0.0014433847],"category_scores_gemma":[0.040222842,0.00045984698,0.00097312225,0.0033553503,0.002021826,0.0049523073,0.0059841266,0.0011652019,0.00018696964],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035628575,0.00010804024,0.5721419,0.0004837982,0.0011388764,0.0004355752,0.0015322315,0.11898026,0.007824581,0.1280026,0.0014479054,0.16754803],"study_design_scores_gemma":[0.000024922598,0.00064266665,0.4668329,0.00052994216,0.0005481037,0.00066081475,0.001638282,0.25021845,0.008131528,0.25826824,0.012283395,0.00022071345],"about_ca_topic_score_codex":0.0027488975,"about_ca_topic_score_gemma":0.0023310503,"teacher_disagreement_score":0.012939759,"about_ca_system_score_codex":0.0011752245,"about_ca_system_score_gemma":0.0008384411,"threshold_uncertainty_score":0.06843287},"labels":[],"label_agreement":null},{"id":"W4410869804","doi":"10.3847/1538-4357/adcba6","title":"Main-sequence Turnoff Stars as Probes of the Ancient Galactic Relic: Chemo-dynamical Analysis of a Pilot Sample","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Stars; Astronomy; Astrophysics; Sample (material); Main sequence; Sequence (biology)","score_opus":0.013228623591535515,"score_gpt":0.25100213561249884,"score_spread":0.23777351202096333,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410869804","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99961084,0.000019486526,0.00008040037,0.0000019064344,4.1224462e-7,0.000005589824,0.00014717784,0.0000026245116,0.00013168674],"genre_scores_gemma":[0.9979432,0.000033876127,0.0004008202,0.000011132725,0.0000043524806,0.000009034586,0.0013709997,0.0000063409857,0.00022009808],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998135,0.000022899261,0.000014093597,0.00007205253,0.00003118894,0.000046299796],"domain_scores_gemma":[0.99948347,0.00005933003,0.00009078987,0.000084055195,0.00010244487,0.00017988418],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027361236,0.0002885712,0.0003287077,0.0013812785,0.00048007292,0.00037022686,0.00024816667,0.0002179256,0.00081137515],"category_scores_gemma":[0.00038058087,0.00015504932,0.00029918016,0.0008394459,0.0003007018,0.00020750861,0.0006915553,0.00013023868,0.00036063298],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013110708,0.00006731831,0.981725,0.000011236659,0.000033914723,0.00013622038,0.0002602792,0.00008529373,0.013695738,0.000023031622,0.00005201316,0.0037789496],"study_design_scores_gemma":[0.0000028199333,0.000058321515,0.9985524,0.0000011044376,0.000011117001,0.000110652836,0.00017742137,0.00015316122,0.00068985415,0.0000095137,0.00023212185,0.0000015996112],"about_ca_topic_score_codex":0.0033810409,"about_ca_topic_score_gemma":0.0065781325,"teacher_disagreement_score":0.0033810409,"about_ca_system_score_codex":0.00021057022,"about_ca_system_score_gemma":0.00013353737,"threshold_uncertainty_score":0.0067227483},"labels":[],"label_agreement":null},{"id":"W4410905056","doi":"10.3847/1538-4357/adceb9","title":"X-Ray and Radio Polarimetry of the Neutron Star Low-mass X-Ray Binary 4U 1728–34","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"National Aeronautics and Space Administration","keywords":"Physics; Neutron star; Astrophysics; X-ray binary; X-ray burster; Astronomy; Binary number; X-ray; Polarimetry; Binary star; Stellar mass loss; Stars; Stellar evolution; Nuclear physics; Scattering; Optics","score_opus":0.006396159645146061,"score_gpt":0.21891285193517848,"score_spread":0.21251669229003242,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410905056","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99821234,0.00015770025,0.00016644003,0.0000141502205,0.000003351252,0.000005137902,0.000114222494,0.00001296656,0.0013137046],"genre_scores_gemma":[0.9981931,0.000069925016,0.0007257511,0.000018439496,0.000010735852,0.0000058145583,0.00049121137,0.000010950303,0.0004742085],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99989223,0.000015308768,0.0000048250163,0.000024476945,0.000035557106,0.000027698823],"domain_scores_gemma":[0.9997284,0.000031710315,0.00010272114,0.000023996701,0.00005562972,0.000057565478],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020522202,0.0003107269,0.00029326658,0.0010445511,0.00047210255,0.00063571514,0.00020150961,0.00027898184,0.001376901],"category_scores_gemma":[0.00035555082,0.00018341729,0.00010482849,0.00054752704,0.0003065232,0.00022580977,0.00057882915,0.00027494782,0.00043793538],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0014854078,0.000104539155,0.29864478,0.00013046313,0.00008700885,0.0014698226,0.0004253853,0.0006726765,0.6765629,0.0005509084,0.00044562828,0.019420467],"study_design_scores_gemma":[0.00005337783,0.00028074448,0.9672523,0.000016299931,0.0000415954,0.00090950803,0.00024517486,0.0008084878,0.0269489,0.00014738146,0.003280408,0.000015854932],"about_ca_topic_score_codex":0.0015890932,"about_ca_topic_score_gemma":0.002617239,"teacher_disagreement_score":0.0015890932,"about_ca_system_score_codex":0.00028087912,"about_ca_system_score_gemma":0.00012638814,"threshold_uncertainty_score":0.0046061873},"labels":[],"label_agreement":null},{"id":"W4410941777","doi":"10.3847/1538-4357/ad7bb8","title":"Statistical Trends in JWST Transiting Exoplanet Atmospheres","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Montreal Clinical Research Institute","funders":"","keywords":"Exoplanet; Physics; Astrobiology; Astronomy; Planet","score_opus":0.008691711747301316,"score_gpt":0.24340474165562873,"score_spread":0.2347130299083274,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410941777","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985904,0.000077995035,0.00030420983,0.00004406312,0.00000439094,0.0000018552628,0.000394352,0.000044570024,0.000538203],"genre_scores_gemma":[0.99920565,0.000022069567,0.00013488933,0.000006463558,0.0000102212425,0.0000018065357,0.00048053794,0.000008432673,0.00012980842],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998275,0.000020710038,0.000014384001,0.00006387638,0.00004813708,0.000025359179],"domain_scores_gemma":[0.9980647,0.00051733863,0.00077005057,0.00013993136,0.0003310083,0.00017695274],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036950083,0.00013268543,0.00016197923,0.0018979794,0.0002006813,0.00056043215,0.00021370857,0.00024488592,0.00093383004],"category_scores_gemma":[0.0022560498,0.00011961066,0.00017155976,0.001432555,0.00032760212,0.00041033243,0.00037765683,0.00026937434,0.00019201866],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000083704996,0.000015168,0.9844593,0.00001721701,0.000073158364,0.0000865253,0.00013611147,0.0008659436,0.008965748,0.00019865579,0.00035308977,0.004745333],"study_design_scores_gemma":[0.0000011311387,0.000018085571,0.9972932,0.0000014893798,0.0000074260843,0.0000476241,0.000062707775,0.0017618375,0.0004780291,0.000072127215,0.00025302224,0.0000034437512],"about_ca_topic_score_codex":0.0028960097,"about_ca_topic_score_gemma":0.0030559304,"teacher_disagreement_score":0.0028960097,"about_ca_system_score_codex":0.00019206372,"about_ca_system_score_gemma":0.00010378729,"threshold_uncertainty_score":0.0057582855},"labels":[],"label_agreement":null},{"id":"W4410967653","doi":"10.3847/1538-4357/adc1c4","title":"A Unified, Physical Framework for Mean Motion Resonances","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Quantum chaos and dynamical systems","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Physics; Motion (physics); Mean motion; Classical mechanics; Astrophysics; Planet","score_opus":0.010469206444308057,"score_gpt":0.2736687537198855,"score_spread":0.2631995472755775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410967653","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.14004423,0.0014549174,0.75935465,0.002819256,0.00041723292,0.000059571103,0.00012856124,0.0003393046,0.09538234],"genre_scores_gemma":[0.9514255,0.0004628317,0.04221098,0.00023014055,0.00027759268,0.00008389719,0.00002636415,0.00007820466,0.005204444],"study_design_codex":"theoretical_or_conceptual","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99974924,0.00009172971,0.000009071114,0.000050123905,0.000060906474,0.000038948852],"domain_scores_gemma":[0.99955434,0.00014294512,0.00007288428,0.00008539942,0.00006928723,0.00007514317],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00069218373,0.0003996047,0.0004306275,0.0010056588,0.0010976363,0.0013953854,0.0009870064,0.0009630371,0.0042424435],"category_scores_gemma":[0.001670293,0.00028258853,0.0005416669,0.00033585387,0.0027045617,0.003128023,0.0015268815,0.0010882694,0.00035076364],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":"theoretical_or_conceptual","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000017163817,0.000002911039,0.000041748273,0.00000476455,0.0000010330796,0.000022826043,0.000025080408,0.004089687,0.0003725702,0.99483055,0.00015367496,0.00045351437],"study_design_scores_gemma":[0.0000045951388,0.000012032498,0.00016125766,0.000007206068,0.0000015519876,0.000042612435,0.000039007835,0.07666355,0.00010593513,0.92104346,0.0019101566,0.000008583999],"about_ca_topic_score_codex":0.000702396,"about_ca_topic_score_gemma":0.0004791764,"teacher_disagreement_score":0.0042424435,"about_ca_system_score_codex":0.0010242215,"about_ca_system_score_gemma":0.0004563983,"threshold_uncertainty_score":0.014192402},"labels":[],"label_agreement":null},{"id":"W4410993892","doi":"10.3847/1538-4357/adcd69","title":"Galaxy Cluster Characterization with Machine Learning Techniques","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"Institut de Valorisation des Données","keywords":"Physics; Cluster (spacecraft); Brightest cluster galaxy; Galaxy cluster; Astrophysics; Galaxy; Astronomy; Characterization (materials science); Type-cD galaxy; Computer science","score_opus":0.0037286173043304025,"score_gpt":0.2017755306948307,"score_spread":0.1980469133905003,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4410993892","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.70766485,0.00038902598,0.27994412,0.00055628654,0.00004203809,0.00022187624,0.0016342727,0.003886672,0.005660962],"genre_scores_gemma":[0.9508107,0.000044612658,0.047558714,0.000038212656,0.000028759167,0.00005586734,0.0007985363,0.000075341224,0.00058923714],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996778,0.00010767403,0.000017232362,0.000088598965,0.00006778499,0.000040879368],"domain_scores_gemma":[0.99790215,0.0008067988,0.00046251516,0.0002858114,0.0004316422,0.0001110786],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009733977,0.0005751569,0.0005422421,0.0031622583,0.00043266613,0.0010252383,0.0010160543,0.00073431287,0.0013973329],"category_scores_gemma":[0.005488418,0.00028570447,0.00064973446,0.0011907269,0.00047783315,0.00078031805,0.00062198355,0.0006350756,0.0005019538],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009727403,0.00006614271,0.0407902,0.00003658723,0.00009304464,0.000052776682,0.0000648002,0.92036813,0.0020318013,0.0022018964,0.0007950034,0.033402383],"study_design_scores_gemma":[0.00000195574,0.0000045395623,0.0031820328,0.0000023241537,0.0000024305941,0.0000048975985,0.0000074748214,0.9954301,0.00034374313,0.00092495413,0.00009125983,0.000004322396],"about_ca_topic_score_codex":0.009289102,"about_ca_topic_score_gemma":0.0059748306,"teacher_disagreement_score":0.009289102,"about_ca_system_score_codex":0.0012409319,"about_ca_system_score_gemma":0.00047209577,"threshold_uncertainty_score":0.018470109},"labels":[],"label_agreement":null},{"id":"W4411077157","doi":"10.3847/1538-4357/add341","title":"From Pretransit to Posteclipse: Investigating the Impact of 3D Temperature, Chemistry, and Dynamics on High-resolution Emission Spectra of the Ultrahot Jupiter WASP-76b","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Agence Nationale de la Recherche","keywords":"Physics; Jupiter (rocket family); Spectral line; Astrobiology; Emission spectrum; Astronomy; Astrophysics; High resolution; Dynamics (music); Hot Jupiter; Spectral resolution; Planet; Remote sensing; Exoplanet; Spacecraft","score_opus":0.004134476551584971,"score_gpt":0.22027871396182783,"score_spread":0.21614423741024286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411077157","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9982173,0.00003868646,0.00074467907,0.00007623852,0.000005527721,0.0000047211174,0.00021144452,0.00006519216,0.0006362581],"genre_scores_gemma":[0.9992218,0.000016269243,0.00039672427,0.000013442874,0.0000019562037,0.0000033755905,0.00021098922,0.000027686165,0.00010777796],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999261,0.000011555405,0.0000020929733,0.000024007604,0.000011064809,0.000025113774],"domain_scores_gemma":[0.9997378,0.00009441732,0.000039176655,0.000028333732,0.000030604475,0.00006959393],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002959966,0.00038341476,0.00023558912,0.00024208023,0.0004547243,0.0007380353,0.0007364942,0.00069186516,0.0011968212],"category_scores_gemma":[0.00079454033,0.00035408276,0.0006294016,0.0002327567,0.00045287737,0.00057147304,0.00045279603,0.0006566547,0.00013803462],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005801757,0.00038236077,0.27321723,0.000082493294,0.000269297,0.0007582047,0.00033159938,0.6819671,0.030902201,0.00190039,0.001408193,0.008200795],"study_design_scores_gemma":[0.000051288425,0.00006865971,0.11587242,0.000010295799,0.00003924167,0.000053662276,0.00010913039,0.87925565,0.0036283147,0.00039098167,0.00049488107,0.000025398791],"about_ca_topic_score_codex":0.033073105,"about_ca_topic_score_gemma":0.020909656,"teacher_disagreement_score":0.033073105,"about_ca_system_score_codex":0.0010126579,"about_ca_system_score_gemma":0.0005400685,"threshold_uncertainty_score":0.06576121},"labels":[],"label_agreement":null},{"id":"W4411133300","doi":"10.3847/1538-4357/add146","title":"Dust Growth in ALMA Rings. II. Dusty Rossby Wave Instability","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; Nanjing University; Academia Sinica; National Science and Technology Council; National Natural Science Foundation of China; Natural Science Foundation of Shanghai","keywords":"Physics; Rossby wave; Instability; Astrophysics; Astronomy; Mechanics; Atmospheric sciences","score_opus":0.010602768163592806,"score_gpt":0.23802160254191776,"score_spread":0.22741883437832494,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411133300","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99640924,0.00015005091,0.0021086144,0.000036503327,0.000004103582,0.000007642957,0.000038368747,0.000035643174,0.0012098418],"genre_scores_gemma":[0.9988438,0.000035101246,0.00074025465,0.0000043552036,0.000005025373,0.0000032196604,0.000028545388,0.0000054843167,0.00033426852],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994314,0.000006912488,0.0000036047568,0.000017341934,0.000012823655,0.000016139275],"domain_scores_gemma":[0.9997905,0.000049139435,0.000076376,0.000024728826,0.00002895074,0.000030246889],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010440242,0.00026426278,0.00014896868,0.0003281482,0.00023377311,0.00042225464,0.00030544764,0.00024722767,0.000533099],"category_scores_gemma":[0.00048686736,0.00012928482,0.00020103829,0.0001782827,0.0002851564,0.00048221753,0.0003352405,0.00022206186,0.00014503418],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00046288176,0.00015435462,0.47108972,0.00020650876,0.00009560462,0.0019058118,0.00087707944,0.07883486,0.3920362,0.012080432,0.00077856326,0.041477926],"study_design_scores_gemma":[0.00004897747,0.00016970276,0.460968,0.000015897289,0.000035104007,0.00053401745,0.0005818862,0.48458835,0.04764591,0.0036435446,0.0017336992,0.00003496365],"about_ca_topic_score_codex":0.002295886,"about_ca_topic_score_gemma":0.0015105997,"teacher_disagreement_score":0.002295886,"about_ca_system_score_codex":0.0003085445,"about_ca_system_score_gemma":0.000119476616,"threshold_uncertainty_score":0.0045651197},"labels":[],"label_agreement":null},{"id":"W4411156900","doi":"10.3847/1538-4357/adda2d","title":"Assessing the Role of Large Fullerenes as Potential Carriers of Infrared Emission Plateaus","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Fullerene Chemistry and Applications","field":"Chemistry","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Physics; Fullerene; Infrared; Astrophysics; Astrobiology; Astronomy; Quantum mechanics","score_opus":0.005376665596444735,"score_gpt":0.26768053443842205,"score_spread":0.2623038688419773,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411156900","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99644357,0.0001504843,0.0018545806,0.000035489797,0.0000023075104,0.0000065777176,0.000040376417,0.00004253876,0.0014240644],"genre_scores_gemma":[0.9994912,0.000027732876,0.00037419001,0.000003921257,8.5023555e-7,0.000005201241,0.000026925858,0.0000063168745,0.000063667314],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994266,0.000007272145,0.0000017741896,0.000010258204,0.000016338501,0.000021724596],"domain_scores_gemma":[0.99970824,0.0001852984,0.000039067374,0.000014941966,0.000028047787,0.000024457579],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00025125002,0.00036766665,0.00020169531,0.00042485545,0.00041830994,0.00045389257,0.00030453256,0.00031425906,0.0016113558],"category_scores_gemma":[0.00079379306,0.0001633617,0.00019926595,0.00018413329,0.00038671817,0.00053304643,0.00031589373,0.00025007705,0.00007596942],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00066982646,0.00026769115,0.021233723,0.00024715817,0.000115127914,0.00085725886,0.00023550508,0.2696869,0.6791169,0.017336093,0.00043489863,0.009798933],"study_design_scores_gemma":[0.00011235846,0.00040438914,0.029117167,0.00004553745,0.000100583464,0.00013892092,0.00021062169,0.71211886,0.25312963,0.0035389615,0.0010351484,0.000047829362],"about_ca_topic_score_codex":0.0014733528,"about_ca_topic_score_gemma":0.0009723133,"teacher_disagreement_score":0.0016113558,"about_ca_system_score_codex":0.00055728405,"about_ca_system_score_gemma":0.0001841052,"threshold_uncertainty_score":0.005390525},"labels":[],"label_agreement":null},{"id":"W4411342333","doi":"10.3847/1538-4357/add334","title":"Thermodynamics of the H <scp>ii</scp> Region Sh2-158 and “Direct” Measurement of Its Turbulence","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Nuclear physics research studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Centre for Research in Astrophysics of Québec","funders":"","keywords":"Physics; Turbulence; Thermodynamics; Statistical physics","score_opus":0.016577389434376533,"score_gpt":0.25100662747519004,"score_spread":0.2344292380408135,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411342333","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9975955,0.000024987734,0.00075749337,0.000014244345,9.115255e-7,0.000004944555,0.00023642361,0.00002141115,0.0013439279],"genre_scores_gemma":[0.999111,0.0000070232395,0.00039008717,0.000005100212,0.0000014885712,0.0000052800256,0.0003424189,0.000007156476,0.00013051183],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99986184,0.000016142998,0.0000034139657,0.00004218772,0.000056009118,0.000020365502],"domain_scores_gemma":[0.999882,0.00003141255,0.000023162955,0.000016718133,0.00002586031,0.000020882406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023338362,0.00016809902,0.00017872931,0.0003813237,0.00025232357,0.00041841163,0.0002907604,0.00013205722,0.0011999707],"category_scores_gemma":[0.0003045985,0.00022187732,0.00020395796,0.00022792895,0.00040374455,0.00031907184,0.00042927946,0.00017560773,0.00015673407],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00035036122,0.00009182405,0.3825888,0.00005819634,0.0001380941,0.00030723755,0.00035507412,0.019416198,0.5870002,0.0014469908,0.00052435807,0.007722732],"study_design_scores_gemma":[0.00002586933,0.00007795942,0.8836304,0.000005120733,0.00001849339,0.000118100106,0.00014225148,0.05274824,0.062171612,0.00035538882,0.0006873616,0.000019289262],"about_ca_topic_score_codex":0.006322106,"about_ca_topic_score_gemma":0.005966063,"teacher_disagreement_score":0.006322106,"about_ca_system_score_codex":0.00049500086,"about_ca_system_score_gemma":0.00016346751,"threshold_uncertainty_score":0.01257062},"labels":[],"label_agreement":null},{"id":"W4411613340","doi":"10.3847/1538-4357/add68a","title":"Filamentary Hierarchies and Superbubbles. I. Characterizing Filament Properties across a Simulated Spiral Galaxy","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Protein filament; Astrophysics; Spiral (railway); Spiral galaxy; Galaxy; Astronomy; Biology","score_opus":0.012999932920588705,"score_gpt":0.25076195169078325,"score_spread":0.23776201877019454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411613340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997971,0.00004269935,0.001404451,0.000015355152,0.0000010906209,0.0000043717087,0.00015800503,0.00004294053,0.00036005615],"genre_scores_gemma":[0.9987488,0.00002134537,0.0009167681,0.0000036753906,7.7466734e-7,0.0000039665483,0.00020736513,0.000007645438,0.000089570116],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99995065,0.000008883634,0.0000029983596,0.000012628262,0.000009329914,0.000015541813],"domain_scores_gemma":[0.9995709,0.00016453014,0.000104249426,0.00005399113,0.000039038918,0.00006721605],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020414747,0.00019663358,0.00016133398,0.0005533126,0.00021852295,0.00031843188,0.0003618635,0.00030450732,0.000725353],"category_scores_gemma":[0.000979536,0.00013418758,0.00030532156,0.00036977872,0.00026028568,0.00029211884,0.00023928887,0.00018462553,0.000068588866],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025142654,0.00010267491,0.1701284,0.0000505661,0.00014614717,0.0003226989,0.00019566147,0.80016863,0.019325191,0.0016359569,0.000352103,0.007320514],"study_design_scores_gemma":[0.000018997363,0.00007702486,0.05550143,0.00000930031,0.000023196062,0.00008768365,0.000053749354,0.9405837,0.0026042354,0.00071711204,0.00031467932,0.000008892099],"about_ca_topic_score_codex":0.007078235,"about_ca_topic_score_gemma":0.005850521,"teacher_disagreement_score":0.007078235,"about_ca_system_score_codex":0.00047008757,"about_ca_system_score_gemma":0.00012533907,"threshold_uncertainty_score":0.014074087},"labels":[],"label_agreement":null},{"id":"W4411616121","doi":"10.3847/1538-4357/add92c","title":"Oort Cloud Formation and Evolution in Star Clusters","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University; Canadian Institute for Theoretical Astrophysics; University of British Columbia","funders":"Natural Sciences and Engineering Research Council of Canada; University of Toronto","keywords":"Physics; Molecular cloud; Astrophysics; Star cluster; Astronomy; Star formation; Protostar; Cloud computing; Stellar evolution; Star (game theory); Astrobiology; Stars","score_opus":0.005983479490965569,"score_gpt":0.23019831740961855,"score_spread":0.224214837918653,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411616121","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99801195,0.000042337135,0.0005130437,0.000050105806,0.0000052520427,0.000008431825,0.00009407131,0.000037753594,0.0012371101],"genre_scores_gemma":[0.9990307,0.000021867902,0.0003866358,0.00002197781,0.0000029548257,0.0000040796745,0.00023232275,0.00001753439,0.00028189097],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9997881,0.000030110197,0.0000068787617,0.00005765155,0.000045652036,0.000071631184],"domain_scores_gemma":[0.9993717,0.0001129496,0.00012901131,0.00006482427,0.00009615097,0.00022532699],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039591378,0.00030961,0.0004416409,0.0005101538,0.0010715051,0.0009684261,0.0007938339,0.00050548284,0.0012684291],"category_scores_gemma":[0.0013644249,0.00023848917,0.00055865134,0.00055857736,0.0006880695,0.00052677776,0.00094650063,0.00043533935,0.00026400818],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006188275,0.00024597728,0.40660256,0.00007780011,0.00028248192,0.00095425476,0.0005333233,0.55024844,0.023430627,0.0060570054,0.0026342806,0.008314364],"study_design_scores_gemma":[0.00017315817,0.00026143686,0.20183755,0.000021919355,0.0000784452,0.00022151005,0.000487252,0.7830738,0.00812975,0.003179936,0.002470512,0.00006476424],"about_ca_topic_score_codex":0.034116622,"about_ca_topic_score_gemma":0.016877811,"teacher_disagreement_score":0.034116622,"about_ca_system_score_codex":0.0022847762,"about_ca_system_score_gemma":0.0007053366,"threshold_uncertainty_score":0.067836106},"labels":[],"label_agreement":null},{"id":"W4411652379","doi":"10.3847/1538-4357/add68e","title":"The 2023 Outburst of the Gaia Alerted EXor Gaia23bab","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Geomagnetism and Paleomagnetism Studies","field":"Biochemistry, Genetics and Molecular Biology","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Magyarország Kormánya; International Max Planck Research School for Advanced Methods in Process and Systems Engineering; Stockholms Universitet; Turun Yliopisto; Háskóli Íslands; Queen's University; Aarhus Universitet; European Commission; Nemzeti Kutatási, Fejlesztési és Innovaciós Alap; Hungarian Scientific Research Fund; Nuclear Safety and Security Commission; International Max Planck Research School for Environmental, Cellular and Molecular Microbiology; HORIZON EUROPE Framework Programme; Space Telescope Science Institute; Agencia Estatal de Investigación; Universitetet i Oslo; Magyar Tudományos Akadémia; University of St Andrews; Queen's University Belfast; National Aeronautics and Space Administration","keywords":"Physics; Astrobiology; Astronomy; Astrophysics","score_opus":0.005185828993155085,"score_gpt":0.22250480649145013,"score_spread":0.21731897749829504,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411652379","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992843,0.00004134023,0.000043436798,0.00003964278,0.000007375567,0.0000028953405,0.00016029301,0.0000069372,0.00041389622],"genre_scores_gemma":[0.99934345,0.000017271674,0.000057563127,0.000019559242,0.0000056507733,0.000002231507,0.0002283106,0.0000020853602,0.0003239506],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999341,0.0000057420248,0.0000033133806,0.00001985408,0.000015318257,0.000021652966],"domain_scores_gemma":[0.9996611,0.000025590887,0.00009108442,0.000021526685,0.000060449245,0.00014034378],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014742924,0.00012311779,0.00019127275,0.0003385407,0.0005264615,0.00040404004,0.00015633168,0.00027733468,0.00083443086],"category_scores_gemma":[0.00039435545,0.000070759146,0.00012306368,0.00020764697,0.00013504851,0.00012399648,0.0003521803,0.00039448857,0.00023233388],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023232317,0.000077930286,0.9579852,0.000027078167,0.000034444303,0.0028838667,0.00090014754,0.00021155122,0.025855327,0.00016197858,0.0009982189,0.010632033],"study_design_scores_gemma":[0.0000017800729,0.000038178332,0.9975418,0.0000039692873,0.000003887948,0.00045804234,0.00026778388,0.00026258721,0.0004978773,0.000025701824,0.0008959237,0.0000026006387],"about_ca_topic_score_codex":0.009054614,"about_ca_topic_score_gemma":0.01864013,"teacher_disagreement_score":0.009054614,"about_ca_system_score_codex":0.00037130687,"about_ca_system_score_gemma":0.00012256046,"threshold_uncertainty_score":0.018003821},"labels":[],"label_agreement":null},{"id":"W4411672041","doi":"10.3847/1538-4357/add68f","title":"The Impact of Initial Composition on Massive Star Evolution and Nucleosynthesis","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Science and Technology Commission of Shanghai Municipality","keywords":"Physics; Nucleosynthesis; Astrophysics; Stellar evolution; Astronomy; Stellar nucleosynthesis; Star (game theory); Stars","score_opus":0.007646817718794877,"score_gpt":0.26187630420509944,"score_spread":0.25422948648630456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411672041","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99753356,0.00010112459,0.0011885865,0.000042498188,0.000008732658,0.0000068249688,0.00023553555,0.00012245531,0.0007606705],"genre_scores_gemma":[0.99852294,0.00003192277,0.00088555965,0.000014710523,0.0000024738458,0.00000425206,0.00039197959,0.00003736947,0.0001088529],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99964213,0.000109653156,0.00002247911,0.00010340686,0.00006316531,0.00005913697],"domain_scores_gemma":[0.996768,0.0023631596,0.00019225465,0.0003064577,0.00021323656,0.00015679668],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012561447,0.00060528977,0.0005352803,0.0005684418,0.00044647645,0.0009760676,0.0006415411,0.0006546576,0.0010658315],"category_scores_gemma":[0.008201222,0.00034749188,0.00063866714,0.00052711327,0.00053078315,0.0006163127,0.0005996193,0.00058210857,0.00018632576],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045165102,0.00012753636,0.14120655,0.00006687653,0.00024007462,0.0003052387,0.000080072474,0.83358353,0.015273402,0.0008851069,0.00033049448,0.0074493964],"study_design_scores_gemma":[0.00010237096,0.00027185056,0.05742691,0.000017444314,0.00010273812,0.00013244552,0.000076261094,0.9104726,0.029734312,0.0010582716,0.0005650645,0.000039821367],"about_ca_topic_score_codex":0.008284794,"about_ca_topic_score_gemma":0.004225355,"teacher_disagreement_score":0.008284794,"about_ca_system_score_codex":0.0006458308,"about_ca_system_score_gemma":0.0003403839,"threshold_uncertainty_score":0.016473174},"labels":[],"label_agreement":null},{"id":"W4411689481","doi":"10.3847/1538-4357/adda3a","title":"Blinded Mock Data Challenge for Gravitational-wave Cosmology. I. Assessing the Robustness of Methods Using Binary Black Hole Mass Spectrum","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Guelph; Perimeter Institute","funders":"Agence Nationale de la Recherche","keywords":"Physics; Cosmology; Gravitational wave; Binary number; Astrophysics; Robustness (evolution); Binary black hole; Gravitation; Astronomy","score_opus":0.12065611363894106,"score_gpt":0.4578499823589734,"score_spread":0.3371938687200323,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411689481","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8091253,0.0016302257,0.17352152,0.0014559191,0.000670506,0.00057804945,0.005211406,0.0021405544,0.005666525],"genre_scores_gemma":[0.9131186,0.000114575276,0.0787776,0.00061364676,0.00012332643,0.00026789814,0.0056485524,0.0003231031,0.0010128011],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.98278576,0.009650654,0.0007373831,0.003514595,0.0028299864,0.00048163088],"domain_scores_gemma":[0.90167654,0.056746785,0.008891859,0.024447436,0.006005841,0.0022316214],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.028464694,0.0010943912,0.0008233696,0.0013129989,0.0014981548,0.002295129,0.0020749755,0.0027896794,0.0016456109],"category_scores_gemma":[0.10307693,0.0004938226,0.0013396159,0.0006757601,0.002566845,0.0024894977,0.0033616421,0.0021815805,0.0006049284],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.010658244,0.0016709289,0.37431964,0.0017776493,0.004331318,0.001098026,0.0019025821,0.35750878,0.03335165,0.066497065,0.027778663,0.11910546],"study_design_scores_gemma":[0.000664904,0.0016998628,0.11528832,0.00043926208,0.0003705005,0.0010610251,0.0009067379,0.75635797,0.04206592,0.059485827,0.021280196,0.00037954067],"about_ca_topic_score_codex":0.0044280267,"about_ca_topic_score_gemma":0.003082738,"teacher_disagreement_score":0.028464694,"about_ca_system_score_codex":0.0013149225,"about_ca_system_score_gemma":0.0013417822,"threshold_uncertainty_score":0.15053749},"labels":[],"label_agreement":null},{"id":"W4411836845","doi":"10.3847/1538-4357/add71a","title":"Milliarcsecond X-Ray Positions and X-Ray Varstrometry for the Strongly Lensed Active Galactic Nucleus HE 0435-1223","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Institut sur la Nutrition et les Aliments Fonctionnels","keywords":"Physics; Active galactic nucleus; Astrophysics; X-ray; Astronomy; Galaxy; Optics","score_opus":0.011732521215496793,"score_gpt":0.24789554218329685,"score_spread":0.23616302096780006,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411836845","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996682,0.00015546964,0.000703415,0.000031372514,0.000005566328,0.0000027677052,0.00042412736,0.00008600132,0.0019092441],"genre_scores_gemma":[0.9981504,0.000037814578,0.0010156534,0.000010455931,0.0000057198777,0.0000021945727,0.0004348629,0.000013738269,0.00032913886],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990356,0.000008831637,0.00000728243,0.000034353525,0.000027488952,0.000018426701],"domain_scores_gemma":[0.999632,0.000048817503,0.00019530502,0.000033923297,0.00004270708,0.000047295427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018640874,0.00017759894,0.00013510196,0.0009917,0.00014526754,0.00045706012,0.00022841454,0.0002356217,0.0013293922],"category_scores_gemma":[0.00037749787,0.000101995945,0.00014747746,0.0006517218,0.00010694271,0.00020351737,0.00019622213,0.00024507885,0.0003315573],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003404059,0.0001133506,0.76162297,0.00006619669,0.00009968281,0.0005527434,0.00035094356,0.0016896139,0.2065448,0.00091160013,0.0009907729,0.026716972],"study_design_scores_gemma":[0.0000035414662,0.000027399457,0.99187964,0.000003374788,0.000010490136,0.00029301885,0.00004874681,0.0015997523,0.0053772717,0.00006606692,0.000685605,0.000005083163],"about_ca_topic_score_codex":0.001687043,"about_ca_topic_score_gemma":0.0034242119,"teacher_disagreement_score":0.001687043,"about_ca_system_score_codex":0.00020650259,"about_ca_system_score_gemma":0.000056966222,"threshold_uncertainty_score":0.0044472814},"labels":[],"label_agreement":null},{"id":"W4411837993","doi":"10.3847/1538-4357/add7d0","title":"Galaxy Zoo CEERS: Bar Fractions Up to <i>z</i> ∼ 4.0","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":21,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Agencia Estatal de Investigación; European Regional Development Fund; Natural Sciences and Engineering Research Council of Canada; Ministerio de Ciencia e Innovación; University of Toronto; National Science Foundation; Fundación Bancaria Caixa d'Estalvis i Pensions de Barcelona; Nuclear Safety and Security Commission; Grantová Agentura České Republiky; National Aeronautics and Space Administration; Canada Research Chairs; Royal Astronomical Society; UK Research and Innovation","keywords":"Physics; Galaxy; Bar (unit); Astrophysics; Astronomy; Galaxy formation and evolution; Meteorology","score_opus":0.008066490999570651,"score_gpt":0.24532872614141316,"score_spread":0.2372622351418425,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411837993","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9826414,0.00016141053,0.0010315237,0.00013125112,0.000011010303,0.000011378912,0.009869371,0.00064698467,0.005495665],"genre_scores_gemma":[0.9845917,0.00004709929,0.0015085859,0.000046100555,0.000015952559,0.000009445144,0.011117622,0.00011737673,0.0025459852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998847,0.00000841359,0.000002456784,0.000039067305,0.000024849793,0.00004051388],"domain_scores_gemma":[0.9992249,0.00010597224,0.00025728438,0.00011227334,0.00012647704,0.00017310624],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026625034,0.00018411169,0.00013301504,0.0011823276,0.0002133828,0.0006262479,0.00019211975,0.00018258758,0.0043397048],"category_scores_gemma":[0.000765168,0.00015853521,0.00020097102,0.0006527241,0.00016433347,0.00047147652,0.00038337437,0.00025996054,0.0009390836],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003127609,0.000051069328,0.9350555,0.00005691998,0.000075078366,0.00021273064,0.00076567655,0.0011341469,0.015994066,0.0012875884,0.014295974,0.030758485],"study_design_scores_gemma":[0.0000045833276,0.0000136150275,0.9925983,0.0000052748946,0.000008716893,0.000058505957,0.0001411994,0.000985356,0.0016586026,0.00017570738,0.0043439786,0.0000061201868],"about_ca_topic_score_codex":0.00927256,"about_ca_topic_score_gemma":0.016696496,"teacher_disagreement_score":0.00927256,"about_ca_system_score_codex":0.00026771548,"about_ca_system_score_gemma":0.00011067891,"threshold_uncertainty_score":0.018437147},"labels":[],"label_agreement":null},{"id":"W4411971052","doi":"10.3847/1538-4357/add930","title":"Dust-obscured Galaxies with Broken Power-law Spectral Energy Distributions Discovered by UNIONS","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Japan Society for the Promotion of Science; University of California, Los Angeles; National Astronomical Observatory of Japan; Deutsches Zentrum für Luft- und Raumfahrt; National Aeronautics and Space Administration; California Institute of Technology; Canadian Space Agency; Jet Propulsion Laboratory; Nuclear Safety and Security Commission; Deutsche Forschungsgemeinschaft; Centre National de la Recherche Scientifique; European Resuscitation Council","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Power law; Spectral energy distribution; Luminous infrared galaxy; Law","score_opus":0.0032295287577017635,"score_gpt":0.1949011952698574,"score_spread":0.19167166651215564,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4411971052","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991786,0.000076061995,0.0003194774,0.000006552325,9.5298356e-7,0.0000019643032,0.000103087215,0.000019781384,0.00029350966],"genre_scores_gemma":[0.99952257,0.000018635028,0.00018768196,0.000006621366,0.000002508032,0.0000010489299,0.00018143324,0.000002960154,0.0000765297],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997845,0.000022501894,0.000011500618,0.00006861058,0.000053077994,0.000059872153],"domain_scores_gemma":[0.9990301,0.00014512446,0.00041280375,0.00012246793,0.0000974288,0.0001921573],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023558733,0.00018297309,0.00029681047,0.0015621738,0.00023623894,0.00051568507,0.00032219346,0.00015143534,0.001271186],"category_scores_gemma":[0.0008534286,0.0001801008,0.00016870984,0.0008897921,0.00045375113,0.00033695216,0.00058338384,0.00021963946,0.00033198902],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008519493,0.000018109438,0.9898992,0.000007446785,0.000019039058,0.00018099503,0.00015994094,0.00008997142,0.0056838263,0.00009400462,0.0001269242,0.0036352973],"study_design_scores_gemma":[0.0000033893105,0.000035871304,0.9973808,0.0000028489187,0.0000071587324,0.00078475237,0.00013591502,0.00039915906,0.0007048274,0.000088830944,0.00045324478,0.0000031292382],"about_ca_topic_score_codex":0.0010546664,"about_ca_topic_score_gemma":0.0013899084,"teacher_disagreement_score":0.0015621738,"about_ca_system_score_codex":0.00019869242,"about_ca_system_score_gemma":0.000056131088,"threshold_uncertainty_score":0.004252553},"labels":[],"label_agreement":null},{"id":"W4412013890","doi":"10.3847/1538-4357/addc71","title":"Forecasting the Fast Radio Burst Population Observed through Galaxy Cluster Lenses","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; McGill University","funders":"","keywords":"Physics; Galaxy cluster; Brightest cluster galaxy; Astronomy; Cluster (spacecraft); Astrophysics; Galaxy; X-shaped radio galaxy; Population; Radio galaxy","score_opus":0.030732842366534195,"score_gpt":0.2495004359874307,"score_spread":0.2187675936208965,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412013890","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9961438,0.000107037384,0.0008360864,0.00006489997,0.0000030464496,0.000020502586,0.0016377929,0.00003564221,0.0011510121],"genre_scores_gemma":[0.9978948,0.000058366488,0.00052901637,0.000012057271,0.0000037495117,0.0000036483684,0.0012806802,0.000003625518,0.00021396742],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99978834,0.000018823266,0.000006362969,0.000056506084,0.00007042383,0.000059565296],"domain_scores_gemma":[0.9981384,0.0003129902,0.00059109065,0.0000993303,0.00044759866,0.000410516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00065455935,0.00026479797,0.0001619851,0.0017155715,0.00036298245,0.00074626895,0.0004463862,0.0003802282,0.0008486252],"category_scores_gemma":[0.0024204983,0.00016482576,0.0001918364,0.0011892408,0.00027125055,0.00046418517,0.0005052415,0.0002220591,0.00023698725],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003559283,0.0000069268913,0.99434644,0.0000049286064,0.000017992006,0.00002843931,0.00003194579,0.0024607698,0.0007463805,0.00011689633,0.00020839123,0.0019952473],"study_design_scores_gemma":[0.0000022635888,0.000017418473,0.9850675,0.000004114083,0.000011180166,0.000021197744,0.00011116785,0.013796537,0.00047372372,0.000091975766,0.0003951698,0.000007762791],"about_ca_topic_score_codex":0.3173427,"about_ca_topic_score_gemma":0.3547764,"teacher_disagreement_score":0.3173427,"about_ca_system_score_codex":0.0024641133,"about_ca_system_score_gemma":0.00089647627,"threshold_uncertainty_score":0.6309911},"labels":[],"label_agreement":null},{"id":"W4412070042","doi":"10.3847/1538-4357/addf30","title":"Carbon-rich Dust Injected into the Interstellar Medium by Galactic WC Binaries Survives for Hundreds of Years","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; European Commission; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; Research Corporation for Science Advancement; European Resuscitation Council; Embry-Riddle Aeronautical University; National Aeronautics and Space Administration","keywords":"Physics; Interstellar medium; Astrophysics; Astronomy; Cosmic dust; Carbon star; Stars; Astrobiology; Galaxy","score_opus":0.006674910470948431,"score_gpt":0.24245934268186364,"score_spread":0.23578443221091522,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412070042","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99924845,0.000069621,0.00008197751,0.000004867098,0.0000018123475,0.0000012217547,0.00009980139,0.000011011135,0.00048128088],"genre_scores_gemma":[0.99947697,0.000017230594,0.0000676445,0.0000038459116,0.0000020929751,0.0000014012361,0.00017275866,0.0000028542447,0.0002550944],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999591,0.0000014211806,0.0000019126446,0.000013911357,0.000008624374,0.000015087738],"domain_scores_gemma":[0.9998895,0.0000085454585,0.00003176434,0.0000123267655,0.00001622079,0.000041733176],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006807838,0.00012234037,0.00015855259,0.00043124286,0.00033364087,0.0004759734,0.00014102757,0.00014848693,0.0009811447],"category_scores_gemma":[0.00012049799,0.000093417766,0.00010016434,0.00021981374,0.00013549998,0.00021306891,0.00025682957,0.00016005228,0.00025415566],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003084196,0.000071007,0.55042607,0.00003832433,0.000076864206,0.00068261405,0.0001823215,0.0004047997,0.439647,0.00015133517,0.00023931576,0.0077719167],"study_design_scores_gemma":[0.0000038914905,0.00006340651,0.9794957,0.000003228461,0.000014272678,0.000269879,0.00017544824,0.0009483163,0.018212657,0.000047707486,0.00076135,0.0000040412606],"about_ca_topic_score_codex":0.0025683602,"about_ca_topic_score_gemma":0.0036866334,"teacher_disagreement_score":0.0025683602,"about_ca_system_score_codex":0.00028209807,"about_ca_system_score_gemma":0.00006671239,"threshold_uncertainty_score":0.0051068068},"labels":[],"label_agreement":null},{"id":"W4412148815","doi":"10.3847/1538-4357/add5f9","title":"GHOST Commissioning Science Results. IV. Chemodynamical Analyses of Milky Way Satellites Sagittarius II and Aquarius II","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Herzberg Institute of Astrophysics; University of Victoria","funders":"","keywords":"Physics; Milky Way; Sagittarius; Astronomy; Astrophysics; Stars","score_opus":0.013471020060218955,"score_gpt":0.2764045173099979,"score_spread":0.26293349724977894,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412148815","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.8537186,0.00065919245,0.0068631903,0.0021133944,0.00030572774,0.0001715278,0.045680635,0.0037768635,0.08671091],"genre_scores_gemma":[0.9510669,0.00012881585,0.013210364,0.00039584798,0.00009356764,0.0000380609,0.025478503,0.0005644724,0.009023491],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99800724,0.0002546734,0.00019364498,0.00029680127,0.0009774851,0.00027015124],"domain_scores_gemma":[0.9795757,0.0038570652,0.0043533784,0.0064182365,0.0041566854,0.0016389235],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004506497,0.00021055859,0.00024791222,0.0045447354,0.00047058906,0.0021313396,0.0004998623,0.00041371267,0.004613444],"category_scores_gemma":[0.008888553,0.00013795159,0.00022230102,0.0033554859,0.00050566427,0.0010499631,0.0011892918,0.0003506926,0.0015179008],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093691034,0.000073946874,0.878776,0.00018696884,0.00011759107,0.0006392825,0.0007349442,0.0022386601,0.010738351,0.008089713,0.028154235,0.06931333],"study_design_scores_gemma":[0.00009638885,0.0001255244,0.8162875,0.00008754453,0.00009498049,0.0006984823,0.00083216775,0.0073176343,0.031615555,0.0039604753,0.13880827,0.0000754535],"about_ca_topic_score_codex":0.0065496503,"about_ca_topic_score_gemma":0.008552458,"teacher_disagreement_score":0.0065496503,"about_ca_system_score_codex":0.0012656166,"about_ca_system_score_gemma":0.0012247325,"threshold_uncertainty_score":0.023832917},"labels":[],"label_agreement":null},{"id":"W4412149018","doi":"10.3847/1538-4357/add34c","title":"A Gravitational-wave-detectable Candidate Type Ia Supernova Progenitor","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Supernova; Gravitational wave; Astrophysics; Astronomy; Progenitor; Progenitor cell; Genetics","score_opus":0.01056843957252485,"score_gpt":0.25195714228514415,"score_spread":0.2413887027126193,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412149018","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974692,0.000057142057,0.0003608248,0.000017775761,0.000006457582,0.000005901987,0.0004201376,0.000037455702,0.0016250525],"genre_scores_gemma":[0.99864537,0.000015068935,0.00037490664,0.000015072615,0.0000044577087,0.0000029798289,0.00054060284,0.0000044418334,0.00039710826],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999542,0.0000021444578,0.0000032239009,0.000019478355,0.000009837356,0.000011089079],"domain_scores_gemma":[0.99988294,0.000010376882,0.00003503454,0.000013543949,0.000015674468,0.000042376152],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010487038,0.00014874229,0.00016904398,0.00038239761,0.00037989795,0.00044979627,0.00017779022,0.0002133242,0.0018116721],"category_scores_gemma":[0.00016261976,0.000083948,0.00012457327,0.00033780272,0.00010719951,0.00013653432,0.00029575825,0.00014697167,0.00048368075],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003092812,0.00007785275,0.742338,0.00003255019,0.00003274684,0.002590122,0.00020153582,0.0002986858,0.24404994,0.0007644165,0.000838045,0.008466878],"study_design_scores_gemma":[0.000012528022,0.00014681838,0.9768003,0.000006418398,0.000023776978,0.0023421727,0.00018329785,0.0017600462,0.01471285,0.00032748567,0.0036744715,0.000009838244],"about_ca_topic_score_codex":0.0027092693,"about_ca_topic_score_gemma":0.0044812635,"teacher_disagreement_score":0.0027092693,"about_ca_system_score_codex":0.00022249843,"about_ca_system_score_gemma":0.00011519528,"threshold_uncertainty_score":0.00606066},"labels":[],"label_agreement":null},{"id":"W4412149047","doi":"10.3847/1538-4357/addc56","title":"Effect of Magnetic Field on the Accretion Phase of Population III Star Formation","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Western University","funders":"","keywords":"Physics; Astrophysics; Accretion (finance); Magnetic field; Intermediate polar; Astronomy; Star formation; Accretion disc; Population; Star (game theory); Phase (matter); Field (mathematics); Stars; White dwarf","score_opus":0.0073324608981158714,"score_gpt":0.2721276950874376,"score_spread":0.26479523418932177,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412149047","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9969009,0.00013907028,0.0003363985,0.00021023896,0.00003355579,0.000009529776,0.00021122851,0.00005270138,0.0021063862],"genre_scores_gemma":[0.9993212,0.00005919708,0.00020929065,0.00004117555,0.000009947289,0.000007463452,0.00015901175,0.000019525669,0.00017308298],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99973613,0.00008670016,0.000014206937,0.000037303358,0.000024704006,0.00010101314],"domain_scores_gemma":[0.99779034,0.0012916353,0.00022808691,0.00010635793,0.0001856101,0.0003979864],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00067626964,0.0006483294,0.0005825393,0.00054200465,0.00064139714,0.0012932633,0.0007582638,0.0009347092,0.002282069],"category_scores_gemma":[0.0055874023,0.0003389867,0.0006183379,0.00044884972,0.00085007836,0.00066483277,0.00068126066,0.001059041,0.00024423303],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010446733,0.0005712271,0.091442704,0.00014424251,0.00034630997,0.0005653655,0.00016230185,0.88334036,0.013082785,0.0021931857,0.0019409573,0.0051659937],"study_design_scores_gemma":[0.0005633084,0.0015853569,0.05795039,0.000081930135,0.00028012716,0.00020848833,0.00056205405,0.9276512,0.007566825,0.0015206998,0.0019202946,0.00010926408],"about_ca_topic_score_codex":0.012255028,"about_ca_topic_score_gemma":0.006996129,"teacher_disagreement_score":0.012255028,"about_ca_system_score_codex":0.0010184064,"about_ca_system_score_gemma":0.0008412116,"threshold_uncertainty_score":0.024367332},"labels":[],"label_agreement":null},{"id":"W4412149280","doi":"10.3847/1538-4357/addbe5","title":"The Milky Way Radial Metallicity Gradient as an Equilibrium Phenomenon: Why Old Stars Are Metal Rich","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":11,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Leibniz-Gemeinschaft; Max-Planck-Institut für Astronomie; Leibniz-Institut für Astrophysik Potsdam; Nanjing University; École Polytechnique Fédérale de Lausanne; Johns Hopkins University; Harvard University; China National Textile and Apparel Council; California Institute of Technology; Alfred P. Sloan Foundation; Flatiron Health; Ohio State University; National Astronomical Observatories, Chinese Academy of Sciences; Carnegie Institution of Washington; Deutsche Forschungsgemeinschaft; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; National Science Foundation","keywords":"Physics; Metallicity; Milky Way; Stars; Astrophysics; Phenomenon; Astronomy; Radial velocity","score_opus":0.01202498201026427,"score_gpt":0.23442896552483217,"score_spread":0.2224039835145679,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412149280","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967656,0.00018884047,0.00102333,0.00019836039,0.000003597293,0.0000018088239,0.00016076204,0.000060623504,0.001597148],"genre_scores_gemma":[0.99930394,0.0000370881,0.00026379369,0.00003423314,0.000004797037,0.0000010089996,0.0000640933,0.000012472042,0.00027863917],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999044,0.000011395542,0.0000052141754,0.000043725177,0.00001638739,0.000018925248],"domain_scores_gemma":[0.9993771,0.00010602174,0.00021799564,0.00007216222,0.00012294222,0.000103765655],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028772646,0.00010593264,0.00018504428,0.00046709314,0.00023208282,0.0011670864,0.00033748843,0.0003218404,0.0014369539],"category_scores_gemma":[0.0016278465,0.000088403605,0.00013428357,0.00044657453,0.0004557918,0.0007434428,0.0003460279,0.00018871341,0.00046778106],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017404449,0.000019909123,0.96239233,0.000034324672,0.00003176509,0.00018087374,0.00047541625,0.0017648744,0.013537591,0.0039559677,0.0010433665,0.01638958],"study_design_scores_gemma":[0.0000093920125,0.000028612063,0.98031723,0.000014572974,0.000019263827,0.00015124265,0.00037684976,0.007548037,0.0041027833,0.005805105,0.0016159691,0.000010871271],"about_ca_topic_score_codex":0.0042847176,"about_ca_topic_score_gemma":0.0050486727,"teacher_disagreement_score":0.0042847176,"about_ca_system_score_codex":0.0005056021,"about_ca_system_score_gemma":0.00013633787,"threshold_uncertainty_score":0.00851953},"labels":[],"label_agreement":null},{"id":"W4412187304","doi":"10.3847/1538-4357/addf49","title":"In Search of the First Stars: An Ultra-compact and Very-low-metallicity Ly<i>α</i> Emitter Deep within the Epoch of Reionization","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Japan Society for the Promotion of Science; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Javna Agencija za Raziskovalno Dejavnost RS; Canadian Foundation for AIDS Research; Canarie; Alliance de recherche numérique du Canada","keywords":"Physics; Reionization; Metallicity; Astrophysics; Epoch (astronomy); Stars; Astronomy; Common emitter; Galaxy; Redshift","score_opus":0.005851356006392107,"score_gpt":0.22043690977581193,"score_spread":0.21458555376941982,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412187304","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9925275,0.00031386924,0.00064499705,0.00025944036,0.000014622001,0.0000080129985,0.00034401217,0.000120689634,0.0057668537],"genre_scores_gemma":[0.99484295,0.00010082547,0.0011666567,0.00019455927,0.000023551273,0.0000024252302,0.0006267951,0.000024466874,0.003017704],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999647,0.000002515673,0.0000013564052,0.000009912288,0.00000890753,0.000012624562],"domain_scores_gemma":[0.99978465,0.000013817085,0.000048146125,0.000020290187,0.000026028754,0.00010717819],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013139451,0.00013205734,0.00013211566,0.00044378373,0.00028274133,0.00041616688,0.000273871,0.00019366191,0.0024864338],"category_scores_gemma":[0.00016724798,0.00006815314,0.00008491754,0.00027842566,0.00012333259,0.00033780452,0.00026231958,0.00020401203,0.00073839974],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039959556,0.00014301307,0.79139626,0.00008867393,0.00005478234,0.002358158,0.0011745566,0.00023573743,0.13208884,0.0013908627,0.008517715,0.06215182],"study_design_scores_gemma":[0.000020263511,0.00020113154,0.9534276,0.000027630504,0.000057730325,0.0015813961,0.0006659745,0.0010829532,0.016952384,0.00053625286,0.025432158,0.0000144231],"about_ca_topic_score_codex":0.002421286,"about_ca_topic_score_gemma":0.007845605,"teacher_disagreement_score":0.0024864338,"about_ca_system_score_codex":0.00017502531,"about_ca_system_score_gemma":0.00007160177,"threshold_uncertainty_score":0.008317947},"labels":[],"label_agreement":null},{"id":"W4412360318","doi":"10.3847/1538-4357/addc70","title":"Asteroseismology of WD J004917.14−252556.81, the Most Massive Pulsating White Dwarf","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Agencia Nacional de Promoción de la Investigación, el Desarrollo Tecnológico y la Innovación; Agencia Nacional de Investigación y Desarrollo; Türkiye Bilimsel ve Teknolojik Araştırma Kurumu; Vlaamse regering; Nuclear Safety and Security Commission; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; Fonds Wetenschappelijk Onderzoek; Consejo Nacional de Investigaciones Científicas y Técnicas; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Ministerio de Asuntos Económicos y Transformación Digital, Gobierno de España; Agència de Gestió d'Ajuts Universitaris i de Recerca; University of Oklahoma; National Science Foundation; Generalitat de Catalunya","keywords":"Asteroseismology; Physics; White dwarf; Astronomy; Astrophysics; Stars","score_opus":0.008518010260191798,"score_gpt":0.2328935334640074,"score_spread":0.2243755232038156,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412360318","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985441,0.00003066522,0.00023894479,0.000016108044,0.0000027083634,0.0000034690415,0.00038149106,0.000021115711,0.0007614244],"genre_scores_gemma":[0.99772173,0.000026676753,0.0004361627,0.000009889865,0.0000034864938,0.0000036711594,0.001172247,0.000005832062,0.00062038243],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995065,0.00000511803,0.0000037207728,0.000018431681,0.000012472511,0.000009608284],"domain_scores_gemma":[0.99983037,0.00001658409,0.00005597905,0.000026771198,0.000020472993,0.000049764396],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017112729,0.00013686436,0.00015550922,0.0006523174,0.0003534856,0.00030654515,0.00015911539,0.00018649621,0.00088110904],"category_scores_gemma":[0.0002515031,0.000084097104,0.00016838264,0.00035121187,0.00015183701,0.00016491898,0.00028375347,0.00015532826,0.00025186234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00028327128,0.000094474795,0.8976091,0.000034106062,0.00004950444,0.0011772395,0.0003461,0.0018993232,0.08105095,0.0003397021,0.0010063117,0.016109956],"study_design_scores_gemma":[0.000005517533,0.000031790296,0.99266136,0.0000039574247,0.0000113234455,0.00020868923,0.00008268509,0.0015331217,0.004034329,0.000071680646,0.0013490674,0.000006465566],"about_ca_topic_score_codex":0.0040902994,"about_ca_topic_score_gemma":0.007695807,"teacher_disagreement_score":0.0040902994,"about_ca_system_score_codex":0.00029743678,"about_ca_system_score_gemma":0.00013794673,"threshold_uncertainty_score":0.008132994},"labels":[],"label_agreement":null},{"id":"W4412386389","doi":"10.3847/1538-4357/ade0bf","title":"SN 2023ixf in the Pinwheel Galaxy M101: From Shock Breakout to the Nebular Phase","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":9,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Grand Équipement National De Calcul Intensif; Tsinghua University; National Aeronautics and Space Administration; California Institute of Technology; University of California Observatories; W. M. Keck Foundation; National Science Foundation","keywords":"Physics; Breakout; Astrophysics; Supernova; Phase (matter); Galaxy; Astronomy; Shock (circulatory); Shock wave; Medicine","score_opus":0.009597450646124495,"score_gpt":0.2611516034769607,"score_spread":0.2515541528308362,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412386389","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99945563,0.00005166458,0.000046757214,0.000009956353,9.4622106e-7,0.0000018691829,0.00011207555,0.000010169304,0.00031099754],"genre_scores_gemma":[0.9995515,0.000018089138,0.000050058727,0.0000074337213,0.0000010676404,0.0000015580632,0.00027166653,0.0000018545263,0.00009676801],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996257,0.0000021044602,0.0000016306036,0.000009698879,0.000007788572,0.000016173255],"domain_scores_gemma":[0.99989927,0.000015852433,0.000031222957,0.000008254652,0.000009918656,0.00003549339],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00007569096,0.00020038741,0.00020541878,0.000578439,0.00029512562,0.00041244683,0.00017415184,0.0003425773,0.0009790036],"category_scores_gemma":[0.00023225682,0.00009239011,0.00019831426,0.00033230442,0.00017616567,0.00015900073,0.00025143192,0.0001825157,0.00019482149],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008774875,0.00010777517,0.9247294,0.00003613064,0.000066905406,0.0026116814,0.00028039498,0.0011158391,0.05350342,0.0003147942,0.000547435,0.015808677],"study_design_scores_gemma":[0.0000068691947,0.000072795985,0.99591655,0.000005388038,0.000007801929,0.0006618987,0.000086516884,0.00080502994,0.0019641172,0.000091434005,0.00037435495,0.0000072738617],"about_ca_topic_score_codex":0.0069043217,"about_ca_topic_score_gemma":0.007098348,"teacher_disagreement_score":0.0069043217,"about_ca_system_score_codex":0.0004850564,"about_ca_system_score_gemma":0.000111985646,"threshold_uncertainty_score":0.013728321},"labels":[],"label_agreement":null},{"id":"W4412415953","doi":"10.3847/1538-4357/addc63","title":"A Catalog of Galactic Supernova Remnants and Supernova Remnant Candidates from the EMU/POSSUM Radio Sky Surveys. I.","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; University of Calgary; University of Alberta","funders":"","keywords":"Physics; Supernova; Sky; Astronomy; Astrophysics; Near-Earth supernova; Supernova remnant; Radio astronomy","score_opus":0.008313965137334756,"score_gpt":0.22785390407642006,"score_spread":0.2195399389390853,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412415953","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.47326788,0.0015913888,0.0027726176,0.00018718098,0.000049744467,0.000387351,0.49172062,0.00213924,0.027884],"genre_scores_gemma":[0.1794038,0.0013107242,0.006030787,0.00010210788,0.000069173446,0.00021628404,0.80156267,0.0002702057,0.01103429],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997024,0.000020444913,0.000068843176,0.000061976796,0.00010301169,0.000043342476],"domain_scores_gemma":[0.9983937,0.00016067395,0.00047758734,0.000250019,0.00043811582,0.00027983738],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00058627204,0.00036976405,0.00033893227,0.009019802,0.00039609216,0.00066314475,0.0004135514,0.00014064672,0.00930533],"category_scores_gemma":[0.0013985976,0.00026504273,0.0003792511,0.007869358,0.000110939276,0.00043858,0.00064653135,0.00014639721,0.0064686453],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003751773,0.0001509971,0.69194716,0.00068390486,0.00013161023,0.0008361488,0.0008227358,0.0006700798,0.009665212,0.0013073587,0.12877274,0.16463688],"study_design_scores_gemma":[0.000023612625,0.000055132226,0.886773,0.00005180779,0.000056229695,0.0005529783,0.00020804422,0.0004976558,0.0020969664,0.00012292052,0.10954792,0.000013699801],"about_ca_topic_score_codex":0.0126379365,"about_ca_topic_score_gemma":0.01946719,"teacher_disagreement_score":0.0126379365,"about_ca_system_score_codex":0.0002568247,"about_ca_system_score_gemma":0.000765816,"threshold_uncertainty_score":0.03112942},"labels":[],"label_agreement":null},{"id":"W4412416129","doi":"10.3847/1538-4357/adddb5","title":"Efficient Ionizers with Low H<b> <i>β</i> </b> + [O <scp>iii</scp>] Equivalent Widths: JADES Spectroscopy of a Peculiar High-redshift Population","year":2025,"lang":"lv","type":"article","venue":"The Astrophysical Journal","topic":"Mass Spectrometry Techniques and Applications","field":"Chemistry","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Science and Technology Facilities Council; European Commission; Royal Society; University of Arizona; Wisconsin Alumni Research Foundation; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; National Research Foundation; UK Research and Innovation; Space Telescope Science Institute; National Science Foundation","keywords":"Physics; Redshift; Spectroscopy; Population; Astrophysics; Astronomy; Galaxy; Medicine","score_opus":0.005062721101544195,"score_gpt":0.24147777213335148,"score_spread":0.2364150510318073,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412416129","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.90266573,0.0012691399,0.046183553,0.0016156037,0.00017384092,0.0001396879,0.0010065839,0.0037632987,0.043182578],"genre_scores_gemma":[0.9428645,0.0007265176,0.026173528,0.0010312148,0.00009428346,0.0001231128,0.00102162,0.0007726913,0.027192516],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99975985,0.000021421738,0.00002277144,0.00006139471,0.0000728748,0.00006173584],"domain_scores_gemma":[0.9996326,0.000077776196,0.000092273396,0.000065249864,0.00008984897,0.000042231295],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004976222,0.00041074984,0.0002862143,0.00050684245,0.00036314563,0.0015485126,0.00080845674,0.00044500586,0.00717123],"category_scores_gemma":[0.00074517704,0.00034233797,0.00015030462,0.00040071172,0.00039453123,0.0013120077,0.0009925762,0.0004106307,0.0027911111],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011939587,0.000096153846,0.009588144,0.000104828905,0.000056144698,0.00025895715,0.00014997242,0.0006880957,0.9580824,0.0024772864,0.005414484,0.02188955],"study_design_scores_gemma":[0.00023991535,0.00037730846,0.015003084,0.00003756094,0.000090518806,0.00070605654,0.00026782035,0.0047872392,0.9447812,0.0007514553,0.03292611,0.000031716867],"about_ca_topic_score_codex":0.00046490808,"about_ca_topic_score_gemma":0.0008965245,"teacher_disagreement_score":0.00717123,"about_ca_system_score_codex":0.0003812243,"about_ca_system_score_gemma":0.00025886833,"threshold_uncertainty_score":0.023990214},"labels":[],"label_agreement":null},{"id":"W4412466875","doi":"10.3847/1538-4357/addd1f","title":"Leaky Dust Traps in Planet-embedded Protoplanetary Disks","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":13,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Montreal Clinical Research Institute; University of Victoria","funders":"","keywords":"Physics; Planet; Protoplanetary disk; Astrobiology; Astronomy; Astrophysics; Planetesimal; Planetary system; Exoplanet","score_opus":0.009102146616530186,"score_gpt":0.24583734731462537,"score_spread":0.23673520069809517,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412466875","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9978618,0.00007276975,0.0009568008,0.00006602296,0.0000077125715,0.0000055817627,0.00008606503,0.00006225704,0.00088103523],"genre_scores_gemma":[0.99943143,0.000023936167,0.00034198986,0.000017669094,0.0000034952575,0.000003305745,0.000053044627,0.000013259689,0.00011186067],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99993634,0.000007893389,0.0000031030077,0.000013476203,0.000013240098,0.0000259489],"domain_scores_gemma":[0.9997423,0.000063560685,0.000052417545,0.00002661131,0.000020126387,0.00009486035],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001173515,0.00030388957,0.00034512847,0.000304178,0.0005501497,0.0009385608,0.00050877663,0.00060892035,0.0012394559],"category_scores_gemma":[0.00063674775,0.00026386502,0.00039822693,0.00016717943,0.00073130504,0.00072564714,0.0008371,0.00050483976,0.00012140452],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005366377,0.00033499397,0.074713,0.00010083083,0.00016227021,0.0009933867,0.00039901852,0.87938017,0.034947496,0.0042195087,0.00079153146,0.0034210745],"study_design_scores_gemma":[0.00014005913,0.00013994657,0.018042358,0.000013118528,0.000018882141,0.0000818572,0.00020932015,0.9760349,0.0029274675,0.0018868552,0.00048174427,0.000023476941],"about_ca_topic_score_codex":0.007053068,"about_ca_topic_score_gemma":0.003103865,"teacher_disagreement_score":0.007053068,"about_ca_system_score_codex":0.00066598057,"about_ca_system_score_gemma":0.0003521699,"threshold_uncertainty_score":0.014024019},"labels":[],"label_agreement":null},{"id":"W4412468753","doi":"10.3847/1538-4357/adde48","title":"Searching for Axion Dark Matter Gegenschein of the Vela Supernova Remnant with FAST","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Vela; Astrophysics; Dark matter; Supernova; Astronomy; Axion; Near-Earth supernova; Astroparticle physics; Supernova remnant; Pulsar; Cosmology","score_opus":0.006382216687788936,"score_gpt":0.22860374664261351,"score_spread":0.22222152995482458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412468753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.996518,0.000057348512,0.0013907973,0.00002357568,0.0000036766048,0.000010176264,0.00023084928,0.000060871254,0.0017047304],"genre_scores_gemma":[0.9979838,0.000017444383,0.0012342702,0.000017102884,0.0000044490794,0.0000048460342,0.00042623313,0.000010732281,0.0003012124],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999856,0.00002072683,0.0000066248194,0.00004065499,0.00002864389,0.00004735884],"domain_scores_gemma":[0.9993693,0.00009751887,0.00018257553,0.00010371053,0.00007847528,0.00016830284],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00055887026,0.00029858036,0.00025017792,0.0010545689,0.00038779373,0.0006649215,0.00030297082,0.00027461277,0.0021982086],"category_scores_gemma":[0.0005255803,0.0002042524,0.00036670125,0.00039450018,0.00021293851,0.00023500492,0.0007654538,0.0002252071,0.00038788398],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00051821594,0.00007750946,0.8318829,0.000038470946,0.00016475741,0.0012393084,0.00025152304,0.0006369577,0.15223964,0.00094366394,0.0004476145,0.011559488],"study_design_scores_gemma":[0.000018335291,0.0002416768,0.9791632,0.000012142325,0.00006366651,0.000903498,0.00034012776,0.0026787128,0.01442232,0.00030246322,0.0018381742,0.000015682483],"about_ca_topic_score_codex":0.0021261284,"about_ca_topic_score_gemma":0.004972889,"teacher_disagreement_score":0.0021982086,"about_ca_system_score_codex":0.00023152455,"about_ca_system_score_gemma":0.0002044036,"threshold_uncertainty_score":0.0073537827},"labels":[],"label_agreement":null},{"id":"W4412473960","doi":"10.3847/1538-4357/adc687","title":"Discovery of a Giant Molecular Cloud at the Midpoint of the Galactic Bar Dust Lanes: M4.7–0.8","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Molecular cloud; Bar (unit); Astrophysics; Midpoint; Astronomy; Cosmic dust; Dust lane; Galactic Center; Cloud computing; Galaxy; Star formation; Stars; Geometry; Meteorology","score_opus":0.005551598312404389,"score_gpt":0.22401759285862996,"score_spread":0.21846599454622556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412473960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99770594,0.000079365585,0.00028048008,0.00008171728,0.000010455143,0.0000063573684,0.00017770955,0.000050095845,0.0016078976],"genre_scores_gemma":[0.9987618,0.000017498804,0.0005796544,0.000055337256,0.000014524239,0.0000034006225,0.00020164497,0.000008355266,0.0003579207],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999393,0.0000022993345,0.0000013177727,0.00001722021,0.000016387727,0.000023504846],"domain_scores_gemma":[0.9997904,0.000014210255,0.000044337292,0.000015606554,0.000027815699,0.00010770649],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009516593,0.00013941788,0.00013790294,0.0004972289,0.00036377818,0.00035070645,0.00039524215,0.00038890736,0.0018391309],"category_scores_gemma":[0.00016899403,0.0001409234,0.0001178294,0.0001586698,0.00028289124,0.00018422863,0.00045980356,0.00028641138,0.000501612],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00040673293,0.00013130684,0.5722297,0.0000571562,0.00007241231,0.00320187,0.0005168823,0.00039575296,0.3984036,0.00078924047,0.0032228706,0.020572426],"study_design_scores_gemma":[0.000027063263,0.00018954897,0.97058064,0.000016572905,0.000038752027,0.0019662993,0.00032261634,0.0012696708,0.018257428,0.00039306225,0.0069241757,0.000014101951],"about_ca_topic_score_codex":0.0014771875,"about_ca_topic_score_gemma":0.0024202126,"teacher_disagreement_score":0.0018391309,"about_ca_system_score_codex":0.00026298544,"about_ca_system_score_gemma":0.000085298496,"threshold_uncertainty_score":0.0061525106},"labels":[],"label_agreement":null},{"id":"W4412506960","doi":"10.3847/1538-4357/ade523","title":"New Field OB and OBe Binaries of the SMC Wing: Observational Properties and Population Modeling","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Solar and Space Plasma Dynamics","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"National Research Foundation of Korea; Deutsche Forschungsgemeinschaft; University of Michigan","keywords":"Physics; Observational study; Wing; Population; Astrophysics; Field (mathematics); Astronomy; Demography; Medicine","score_opus":0.024482252159749793,"score_gpt":0.2308485098194684,"score_spread":0.2063662576597186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412506960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998398,0.000035820533,0.0010121309,0.000010105775,8.552536e-7,0.000006652155,0.00013086971,0.000013469234,0.00039206867],"genre_scores_gemma":[0.99906677,0.000015871501,0.0004191963,0.000003828681,0.0000029766231,0.000003974609,0.00036020647,0.0000038762773,0.00012336108],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989367,0.000020008247,0.0000051582806,0.000040850155,0.000017972123,0.000022352786],"domain_scores_gemma":[0.9995839,0.00010863963,0.00010017567,0.000055917717,0.000051236842,0.00010007178],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00060078857,0.00025254115,0.00033099356,0.0009101268,0.00048470098,0.0006014491,0.00045851304,0.00026750474,0.0012234587],"category_scores_gemma":[0.0008713125,0.00016784757,0.00032248354,0.00046009032,0.00022729764,0.00037206546,0.00045581683,0.00016413412,0.00026558278],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000093429924,0.00006822968,0.98026043,0.0000057711686,0.000039134364,0.000054586868,0.00007076829,0.01285945,0.00073902495,0.00047006583,0.00016726136,0.005171748],"study_design_scores_gemma":[0.00003067993,0.00008402082,0.6333703,0.000009138678,0.000038637358,0.00013634883,0.00013250211,0.36358595,0.0007747313,0.0009965836,0.00082953135,0.000011623376],"about_ca_topic_score_codex":0.008806529,"about_ca_topic_score_gemma":0.0077224937,"teacher_disagreement_score":0.008806529,"about_ca_system_score_codex":0.00043803683,"about_ca_system_score_gemma":0.0001741774,"threshold_uncertainty_score":0.017510533},"labels":[],"label_agreement":null},{"id":"W4412507030","doi":"10.3847/1538-4357/ade14c","title":"A Multi-wavelength Characterization of the 2023 Outburst of MAXI J1807+132: Manifestations of Disk Instability and Jet Emission","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Astrophysics Science Division; Agencia Estatal de Investigación; Goddard Space Flight Center; European Southern Observatory; Ministerio de Ciencia, Innovación y Universidades; Nuclear Safety and Security Commission; Tamkeen; European Commission; University of Warwick; University of Leicester; HORIZON EUROPE Framework Programme; New York University Abu Dhabi; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Instability; Jet (fluid); Wavelength; Astronomy; Characterization (materials science); Emission spectrum; Spectral line; Optics; Mechanics","score_opus":0.013217130269154154,"score_gpt":0.24340424417266127,"score_spread":0.2301871139035071,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412507030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998933,0.00006161599,0.00010701175,0.000011391096,0.0000025525699,0.0000052505916,0.00016833497,0.0000115366975,0.00069938187],"genre_scores_gemma":[0.9990146,0.000038188344,0.00020736,0.000014345029,0.000010686378,0.000006855463,0.0004608591,0.000007851751,0.00023913445],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995553,0.000004122887,0.0000025011223,0.000013182622,0.000010202559,0.000014393294],"domain_scores_gemma":[0.9996729,0.00003208502,0.00012702947,0.000021947752,0.000035320692,0.00011077193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014270103,0.00023194547,0.00020478868,0.0007025285,0.00034878196,0.000359088,0.00016270195,0.00019992537,0.0009651795],"category_scores_gemma":[0.00024982158,0.000118026524,0.00013202209,0.0004070121,0.00015651036,0.00016166075,0.0003917513,0.0002704851,0.00026095833],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049915334,0.00012610118,0.7699302,0.000051627994,0.00004040168,0.0011323646,0.000536976,0.00013840884,0.21883923,0.00011484392,0.00033539912,0.008255278],"study_design_scores_gemma":[0.0000021759643,0.00004770737,0.99829215,0.0000019719484,0.0000043360387,0.00020734781,0.000073396746,0.00008958297,0.0010503974,0.000015124524,0.00021368689,0.0000020800733],"about_ca_topic_score_codex":0.0014226625,"about_ca_topic_score_gemma":0.0033257122,"teacher_disagreement_score":0.0014226625,"about_ca_system_score_codex":0.00014692164,"about_ca_system_score_gemma":0.00007312865,"threshold_uncertainty_score":0.0032288432},"labels":[],"label_agreement":null},{"id":"W4412583761","doi":"10.3847/1538-4357/ade0b3","title":"The Gravity Collective: A Comprehensive Analysis of the Electromagnetic Search for the Binary Neutron Star Merger GW190425","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"H2020 European Research Council; PAZY Foundation; Israel Science Foundation; United States - Israel Binational Science Foundation","keywords":"Physics; Neutron star; Astrophysics; Astronomy; Binary number; Gravitational wave; Binary star; Star (game theory); Stars","score_opus":0.011861610602937566,"score_gpt":0.3263407660431825,"score_spread":0.31447915544024496,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412583761","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9964026,0.00015468714,0.0005415706,0.00006525338,0.0000023436355,0.000007931193,0.00092555856,0.000067596295,0.0018322669],"genre_scores_gemma":[0.99442333,0.00007953792,0.0008686074,0.00002882456,0.000011711063,0.0000070218375,0.004195043,0.000036612448,0.00034940825],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997242,0.00004362646,0.000010443314,0.000071406044,0.00009779699,0.00005240675],"domain_scores_gemma":[0.9994229,0.00013289358,0.00016999779,0.00007773542,0.00006147583,0.0001349436],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046418648,0.00034424354,0.00034235057,0.0026372643,0.0004016692,0.0006555629,0.00035652614,0.00020031673,0.00087816245],"category_scores_gemma":[0.0013522202,0.00016612018,0.00047937673,0.0019951616,0.00029814287,0.00041464524,0.0011707011,0.00019823464,0.00022174366],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030914828,0.00011525858,0.93994755,0.000079988415,0.00044876305,0.00076022843,0.00040243898,0.017435852,0.008953854,0.0018929241,0.0038064055,0.02584758],"study_design_scores_gemma":[0.000021825237,0.00009136932,0.97135353,0.000013422347,0.00009191827,0.00023201814,0.0003969287,0.022117248,0.0011519688,0.0008349977,0.003668822,0.00002592978],"about_ca_topic_score_codex":0.0131710945,"about_ca_topic_score_gemma":0.017970031,"teacher_disagreement_score":0.0131710945,"about_ca_system_score_codex":0.0003853859,"about_ca_system_score_gemma":0.00028966804,"threshold_uncertainty_score":0.02618891},"labels":[],"label_agreement":null},{"id":"W4412603619","doi":"10.3847/1538-4357/addf2e","title":"The Centre of Attention: A Powerful Radio Galaxy Pinpoints a Near-infrared-dark Protocluster at <i>z</i> ∼ 3.9","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Galaxy; Infrared; Astronomy; Radio galaxy; Galaxy formation and evolution","score_opus":0.004003727662353292,"score_gpt":0.20680035564826516,"score_spread":0.20279662798591186,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412603619","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9955818,0.00008921357,0.0006010476,0.00012292115,0.000012205108,0.000006264881,0.00008181999,0.000064951746,0.0034398015],"genre_scores_gemma":[0.9984257,0.000019813982,0.00058608915,0.00009042227,0.000010140638,0.0000024407934,0.00007569234,0.0000067396136,0.00078308367],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999566,0.0000026291852,0.0000014888241,0.00001128978,0.000013002615,0.000014989714],"domain_scores_gemma":[0.9998136,0.000019063109,0.000057177145,0.000020769203,0.000023036644,0.00006634227],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000077797326,0.0001331347,0.00011296379,0.00038940483,0.00032390832,0.00041237907,0.00034497422,0.00022794245,0.002740749],"category_scores_gemma":[0.00024797485,0.00009155195,0.000110980116,0.00015280738,0.00031871008,0.00022674612,0.0005244091,0.00020910926,0.00055681734],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00049537345,0.00006478111,0.73624814,0.000053637967,0.000061919236,0.017933723,0.0028442037,0.0001661645,0.19763465,0.0018150033,0.003908957,0.038773447],"study_design_scores_gemma":[0.000012640277,0.00017229618,0.9601743,0.000022109565,0.000032322063,0.01367028,0.0011026413,0.0007457792,0.015156417,0.0006377415,0.00825997,0.000013415719],"about_ca_topic_score_codex":0.0016452867,"about_ca_topic_score_gemma":0.0025291846,"teacher_disagreement_score":0.002740749,"about_ca_system_score_codex":0.0002052277,"about_ca_system_score_gemma":0.000067875415,"threshold_uncertainty_score":0.0091686845},"labels":[],"label_agreement":null},{"id":"W4412668605","doi":"10.3847/1538-4357/ade787","title":"Early and Extensive Ultraviolet through Near Infrared Observations of the Intermediate-luminosity Type Iax Supernovae 2024pxl","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Agencia Nacional de Investigación y Desarrollo; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Ohio State University; Queen's University; European Commission; Gordon and Betty Moore Foundation; Nuclear Safety and Security Commission; Space Telescope Science Institute; Alfred P. Sloan Foundation; Queen's University Belfast; National Aeronautics and Space Administration; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Physics; Supernova; Astrophysics; Luminosity; Infrared; Astronomy; Ultraviolet; Galaxy; Optics","score_opus":0.01505477995100679,"score_gpt":0.239713096053542,"score_spread":0.2246583161025352,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412668605","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998351,0.000037398044,0.00017619156,0.000006937816,0.0000019066972,0.000003885206,0.00018918792,0.000018236036,0.0012153666],"genre_scores_gemma":[0.99756336,0.000037729933,0.00050420745,0.00001669574,0.0000066899647,0.000007358695,0.0010097356,0.0000059480335,0.00084821455],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999374,0.000004868889,0.0000033582858,0.000013570287,0.000024886132,0.000015930618],"domain_scores_gemma":[0.99984324,0.000010172841,0.000044867258,0.000011062351,0.00002760846,0.00006300064],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015670808,0.00021220157,0.00017078694,0.0007436965,0.00039134163,0.00031656938,0.00015869462,0.00017802246,0.00096787454],"category_scores_gemma":[0.00014855179,0.00011440589,0.00019185542,0.00029823981,0.0001436011,0.00019444921,0.00050111936,0.00022368193,0.00035197288],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004163827,0.0001630382,0.8220116,0.00003664711,0.00007645661,0.0011847869,0.000280213,0.00033732274,0.16210145,0.0001679379,0.0005560003,0.01266811],"study_design_scores_gemma":[0.0000045319457,0.000104349325,0.995717,0.0000031111208,0.0000082873385,0.00043499,0.00008627325,0.00023345216,0.0025074438,0.000030662177,0.0008664627,0.0000034107738],"about_ca_topic_score_codex":0.001670068,"about_ca_topic_score_gemma":0.0036874271,"teacher_disagreement_score":0.001670068,"about_ca_system_score_codex":0.00018571774,"about_ca_system_score_gemma":0.00010276947,"threshold_uncertainty_score":0.003320694},"labels":[],"label_agreement":null},{"id":"W4412685630","doi":"10.3847/1538-4357/ade793","title":"Unified Weak Lensing Constraints on the Evolution of the Mass–X-Ray Luminosity Relation for Galaxy Clusters","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"Conselho Nacional de Desenvolvimento Científico e Tecnológico; Financiadora de Estudos e Projetos; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Fundação de Amparo à Pesquisa do Estado de São Paulo","keywords":"Physics; Astrophysics; Luminosity; Galaxy cluster; Weak gravitational lensing; Astronomy; Galaxy; Galaxy groups and clusters; Redshift","score_opus":0.009179821667819084,"score_gpt":0.2136339158574321,"score_spread":0.20445409418961302,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412685630","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98528016,0.00037897585,0.009334633,0.00010046094,0.000005549887,0.000008628991,0.0009876756,0.00020390394,0.0037001863],"genre_scores_gemma":[0.99705505,0.00007083371,0.001631052,0.00002063926,0.000011979152,0.000004699378,0.0008932932,0.000041681164,0.0002707615],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994623,0.00011665544,0.0000366962,0.00015377576,0.00015194512,0.00007866415],"domain_scores_gemma":[0.994451,0.0021325147,0.0011028597,0.001067834,0.00081871066,0.00042713748],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0021548436,0.00054559717,0.0004556094,0.0021184597,0.00049968244,0.0018076848,0.0006320113,0.00034711722,0.0023811802],"category_scores_gemma":[0.0058445805,0.00037072343,0.00059832336,0.0009977929,0.00054954074,0.00073921954,0.0011115521,0.00038922616,0.0005471094],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00034445283,0.00005988639,0.86121607,0.000130306,0.00037063987,0.00035676904,0.0004119395,0.06276202,0.029649133,0.016501956,0.0018060384,0.026390843],"study_design_scores_gemma":[0.000020358346,0.00006712302,0.8796976,0.000039056817,0.0000762358,0.00012406243,0.00018248732,0.10557888,0.005408398,0.006520312,0.0022341516,0.000051424482],"about_ca_topic_score_codex":0.009720592,"about_ca_topic_score_gemma":0.009274566,"teacher_disagreement_score":0.009720592,"about_ca_system_score_codex":0.0008026896,"about_ca_system_score_gemma":0.0003603318,"threshold_uncertainty_score":0.019327998},"labels":[],"label_agreement":null},{"id":"W4412729670","doi":"10.3847/1538-4357/add2ee","title":"Dust in the Smith Cloud? A UV Investigation into the Smith Cloud’s Gas-phase Abundance Patterns","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Okanagan University College; University of British Columbia, Okanagan Campus; Dominion Astrophysical Observatory; Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute","keywords":"Physics; Cloud computing; Abundance (ecology); Astrophysics; Astronomy; Gas phase; Thermodynamics","score_opus":0.011309078636670642,"score_gpt":0.2650777110923123,"score_spread":0.2537686324556417,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412729670","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99873227,0.000035377627,0.00004872382,0.000016210875,9.678197e-7,0.00000263684,0.00011552483,0.000004342019,0.0010439318],"genre_scores_gemma":[0.99941397,0.000024089475,0.000114914714,0.000011431348,0.0000037796192,0.0000011271699,0.0001454352,0.0000018643819,0.00028341266],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995244,0.00000294206,0.000001984162,0.000011094772,0.000015201808,0.000016217326],"domain_scores_gemma":[0.9998147,0.000022798877,0.000054823675,0.000011271848,0.000039623737,0.000056909394],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006631698,0.00006806987,0.00012628357,0.0006531834,0.00034594396,0.0003026535,0.00013774431,0.00009390981,0.0014851339],"category_scores_gemma":[0.00017432746,0.000063659114,0.000062686464,0.00043724416,0.00022668774,0.00017384689,0.00017940544,0.000091800925,0.00014522072],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016108878,0.00004299248,0.931731,0.00001360506,0.000021859663,0.00044305774,0.0003053944,0.00020114466,0.058691293,0.00023981222,0.0004032,0.0077454573],"study_design_scores_gemma":[0.0000033674137,0.000024946827,0.9947141,0.000002539277,0.000004175766,0.00012309097,0.00024762217,0.0005115757,0.003316173,0.00004811709,0.0010023377,0.000001972765],"about_ca_topic_score_codex":0.02041282,"about_ca_topic_score_gemma":0.02444633,"teacher_disagreement_score":0.02041282,"about_ca_system_score_codex":0.00044643495,"about_ca_system_score_gemma":0.00014108475,"threshold_uncertainty_score":0.04058802},"labels":[],"label_agreement":null},{"id":"W4412846206","doi":"10.3847/1538-4357/ade709","title":"Peering into the Heart of Darkness with VLBA: Radio-quiet Active Galactic Nucleus in the JWST North Ecliptic Pole Time-domain Field","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Ecliptic; Peering; QUIET; Astronomy; Active galactic nucleus; Astrophysics; Nucleus; Magnetic field; Galaxy; Solar wind","score_opus":0.003512257555623479,"score_gpt":0.20424007868118157,"score_spread":0.2007278211255581,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412846206","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98965305,0.00026575083,0.00057839626,0.00066192803,0.00009174151,0.000025484396,0.0008338256,0.0001057817,0.0077840155],"genre_scores_gemma":[0.9956167,0.00011856763,0.00058486225,0.00012772281,0.00009257484,0.000007055128,0.0010710701,0.000028695693,0.0023528738],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993734,0.00013198495,0.00003578123,0.00011894454,0.00022459109,0.000115387185],"domain_scores_gemma":[0.9938075,0.00104117,0.0016137494,0.0007495962,0.0014219221,0.0013661685],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0009451754,0.00011080279,0.0001623206,0.0014881926,0.00068803766,0.0011543994,0.00034526407,0.00021623314,0.0045988616],"category_scores_gemma":[0.006590237,0.00007976697,0.00006157798,0.00078978244,0.00048566805,0.00090746494,0.0011820614,0.000221709,0.0009888017],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000101027355,0.000041767285,0.92993057,0.000035223275,0.000017809341,0.00034482768,0.0019458514,0.00007558738,0.0059360736,0.00027534275,0.009130051,0.052165974],"study_design_scores_gemma":[0.0000050973936,0.000029532515,0.9840785,0.000016980264,0.000004335027,0.00017897443,0.0022976217,0.00027437683,0.0007578779,0.00018609173,0.012162575,0.000007936767],"about_ca_topic_score_codex":0.009781912,"about_ca_topic_score_gemma":0.022904556,"teacher_disagreement_score":0.009781912,"about_ca_system_score_codex":0.00049257424,"about_ca_system_score_gemma":0.00039900155,"threshold_uncertainty_score":0.01944995},"labels":[],"label_agreement":null},{"id":"W4412846212","doi":"10.3847/1538-4357/ade9b5","title":"The Evolution of Substructure during Star Cluster Assembly","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"","keywords":"Physics; Substructure; Cluster (spacecraft); Star (game theory); Star cluster; Astrophysics; Astronomy; Stars","score_opus":0.003793024081595517,"score_gpt":0.22200789377795616,"score_spread":0.21821486969636064,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412846212","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99852365,0.000030976385,0.0005459195,0.000037712118,0.0000048518705,0.0000054576753,0.000060418995,0.000028445245,0.00076248095],"genre_scores_gemma":[0.99938285,0.000014743495,0.00031247767,0.000009114121,0.0000015834402,0.0000034018742,0.00007836378,0.000010599672,0.00018680062],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998653,0.00002603962,0.000006454983,0.000022300263,0.0000251254,0.000054711072],"domain_scores_gemma":[0.9991665,0.00030384184,0.0001555664,0.00008277504,0.00010433931,0.00018699311],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003755041,0.00032395677,0.0003497262,0.00032112838,0.0006772562,0.0010099342,0.00059041375,0.00057813857,0.001144216],"category_scores_gemma":[0.0020277991,0.0002973438,0.0004195591,0.00031815027,0.0006636961,0.0005271286,0.00066674716,0.0006133985,0.00012530501],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00032214512,0.00018217384,0.07514516,0.000037399306,0.00013282771,0.00035657635,0.0002689327,0.9013343,0.016623596,0.0021128878,0.00034513004,0.003138954],"study_design_scores_gemma":[0.00006958118,0.00023257475,0.039748605,0.000013518418,0.00003967423,0.000080110294,0.00013776011,0.95363617,0.004863736,0.0006454332,0.0005028024,0.000030008545],"about_ca_topic_score_codex":0.015490197,"about_ca_topic_score_gemma":0.009984527,"teacher_disagreement_score":0.015490197,"about_ca_system_score_codex":0.0010861605,"about_ca_system_score_gemma":0.0005499631,"threshold_uncertainty_score":0.030800104},"labels":[],"label_agreement":null},{"id":"W4412912292","doi":"10.3847/1538-4357/ade443","title":"Timescales of Polycyclic Aromatic Hydrocarbon and Dust Continuum Emission from Gas Clouds Compared to Molecular Gas Cloud Lifetimes in PHANGS-JWST Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"Australian Research Council; Deutsche Forschungsgemeinschaft; National Aeronautics and Space Administration","keywords":"Physics; Molecular cloud; Galaxy; Polycyclic aromatic hydrocarbon; Astrophysics; Cosmic dust; Interstellar cloud; Astronomy; Star formation; Hydrocarbon; Interstellar medium; Astrobiology; Stars","score_opus":0.005606878208378861,"score_gpt":0.23308327241243387,"score_spread":0.22747639420405502,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412912292","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987551,0.000099318706,0.00010100568,0.000007921334,0.0000019095694,0.0000040154396,0.00044913142,0.000019902896,0.00056164566],"genre_scores_gemma":[0.9985121,0.000042280986,0.00015231152,0.000009133995,0.000005292767,0.0000061651704,0.0011175483,0.0000068969234,0.00014829381],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999027,0.000004408559,0.0000060361845,0.000043965323,0.000015361884,0.00002743451],"domain_scores_gemma":[0.9995585,0.000053719177,0.00015946596,0.00004045913,0.000050664232,0.00013719831],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015719641,0.00016129276,0.00015288113,0.001130515,0.00020999098,0.00048805668,0.00023799535,0.00019398218,0.00077233464],"category_scores_gemma":[0.0005756738,0.00013353405,0.00019655524,0.00047263494,0.00021544822,0.00038473544,0.00037782785,0.00016322982,0.00020541565],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000119060176,0.000032005824,0.9683441,0.000021735594,0.00004148938,0.000098047065,0.00028715745,0.00037906013,0.024675108,0.00012990736,0.00022540514,0.005646892],"study_design_scores_gemma":[0.0000017597318,0.000012359936,0.9987172,0.0000016806842,0.000004324391,0.000029144201,0.000042344833,0.00036228044,0.0006228314,0.000026334641,0.0001779976,0.0000016424449],"about_ca_topic_score_codex":0.004627345,"about_ca_topic_score_gemma":0.004985824,"teacher_disagreement_score":0.004627345,"about_ca_system_score_codex":0.00036019544,"about_ca_system_score_gemma":0.000077845856,"threshold_uncertainty_score":0.009200811},"labels":[],"label_agreement":null},{"id":"W4412924994","doi":"10.3847/1538-4357/ade232","title":"A Map of the Outer Gas Disk of the Galaxy with Direct Distances from Young Stars","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Stars; Astronomy; Galaxy","score_opus":0.004799984931444366,"score_gpt":0.19856644555692626,"score_spread":0.1937664606254819,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412924994","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9859767,0.000235217,0.0047352063,0.00005027228,0.000008947772,0.000014880242,0.0030479007,0.0002251737,0.0057056868],"genre_scores_gemma":[0.9928389,0.00006356228,0.005245829,0.0000065491245,0.000009883546,0.000005085765,0.0012811758,0.000016891678,0.0005321761],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999577,0.0000052096116,0.0000014964385,0.000017614717,0.000011130269,0.0000068328495],"domain_scores_gemma":[0.99973375,0.000051216775,0.00006291401,0.000030661926,0.00006224619,0.000059241855],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006992876,0.0001397024,0.00009564338,0.0012115083,0.00017684122,0.00035229366,0.00016589889,0.00017371764,0.002683376],"category_scores_gemma":[0.00046356348,0.00009310437,0.00013266974,0.00084607746,0.00009773059,0.00018659921,0.00031253032,0.000112235706,0.00065594976],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00068221794,0.00013503278,0.7775297,0.0001485284,0.00018065143,0.00064365205,0.0006372377,0.020622574,0.083489895,0.002326861,0.0032653168,0.11033829],"study_design_scores_gemma":[0.000022950939,0.00005993116,0.96729785,0.000014598176,0.0000323545,0.00030125212,0.00012225246,0.022133987,0.004284487,0.0006993909,0.0050207973,0.000010147226],"about_ca_topic_score_codex":0.004869152,"about_ca_topic_score_gemma":0.0055370023,"teacher_disagreement_score":0.004869152,"about_ca_system_score_codex":0.00021699442,"about_ca_system_score_gemma":0.00014399599,"threshold_uncertainty_score":0.009681642},"labels":[],"label_agreement":null},{"id":"W4412993381","doi":"10.3847/1538-4357/ade997","title":"Infant Core-collapse Supernovae with Circumstellar Interactions from KMTNet. I. Luminous Transitional Case of KSP-SN-2022c","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Korea Astronomy and Space Science Institute","keywords":"Physics; Supernova; Astrophysics; Core (optical fiber); Astronomy; Optics","score_opus":0.010155452538716074,"score_gpt":0.24066472261984284,"score_spread":0.23050927008112676,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412993381","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99884194,0.000040242016,0.00011560498,0.000017869996,0.0000029813564,0.0000051305874,0.000047490357,0.000007488584,0.00092127203],"genre_scores_gemma":[0.99975497,0.000010434506,0.000049945207,0.000007317009,0.000003389786,0.0000014220522,0.00007694793,0.0000017451503,0.0000937384],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999013,0.000009894915,0.00000899941,0.000022423093,0.00001787759,0.00003956796],"domain_scores_gemma":[0.99975425,0.000017576971,0.000053228403,0.00002451302,0.0000082927945,0.00014205779],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015095656,0.00037410134,0.0002446066,0.00046566405,0.0005980594,0.00056192017,0.00047019447,0.0003824556,0.0011936675],"category_scores_gemma":[0.00045095134,0.00015284309,0.00032321425,0.0002653221,0.00037423382,0.00013680723,0.0006137491,0.00033654924,0.0002079386],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011353326,0.00022936339,0.8738344,0.000037645845,0.00009014007,0.09945506,0.0002760278,0.003104182,0.012821285,0.0027455825,0.00037757703,0.005893304],"study_design_scores_gemma":[0.00009965531,0.00060764834,0.88843983,0.000022645261,0.00005765149,0.08897313,0.00068213325,0.014359929,0.0029812746,0.00207991,0.0016655043,0.000030614417],"about_ca_topic_score_codex":0.0033990717,"about_ca_topic_score_gemma":0.004496533,"teacher_disagreement_score":0.0033990717,"about_ca_system_score_codex":0.00040565673,"about_ca_system_score_gemma":0.00023249035,"threshold_uncertainty_score":0.0067585707},"labels":[],"label_agreement":null},{"id":"W4412993668","doi":"10.3847/1538-4357/ade9a4","title":"Identifying Dwarfs of MC Analog GalaxiEs (ID-MAGE): The Search for Satellites around Low-mass Hosts","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University; University of Toronto","funders":"","keywords":"Physics; Galaxy; Astrophysics; Low Mass; Astronomy; Stars","score_opus":0.012864150243199077,"score_gpt":0.2609131576793927,"score_spread":0.24804900743619362,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412993668","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985253,0.000084292435,0.00040286948,0.0000074969985,8.491547e-7,0.0000067911615,0.00046777597,0.000030903648,0.00047380276],"genre_scores_gemma":[0.9979419,0.000029935765,0.0010454769,0.000008267071,0.0000027522876,0.0000031394188,0.0008108788,0.0000032652201,0.00015443118],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997801,0.00003169914,0.000012842883,0.00006128247,0.00007270842,0.000041317133],"domain_scores_gemma":[0.99858236,0.00024063408,0.00037033705,0.00021134138,0.00020324503,0.00039215488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0004592317,0.00019640013,0.00019639263,0.0018424637,0.00025091966,0.0004905349,0.00026335756,0.00013560106,0.0006878302],"category_scores_gemma":[0.0011581393,0.000087717795,0.00016312292,0.0007240723,0.00022020435,0.0002128577,0.0005816075,0.00010614538,0.00023106739],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006719187,0.00001654186,0.9831291,0.000018131781,0.00002358409,0.000058844034,0.0000802069,0.00020955282,0.007151931,0.00006770278,0.0001611946,0.009016133],"study_design_scores_gemma":[0.00000420869,0.00006258357,0.99431396,0.00000565798,0.000019740364,0.00018882548,0.00013152533,0.0011363224,0.0032743914,0.000052946027,0.00080612686,0.0000036382244],"about_ca_topic_score_codex":0.0025713034,"about_ca_topic_score_gemma":0.0049383272,"teacher_disagreement_score":0.0025713034,"about_ca_system_score_codex":0.00016829645,"about_ca_system_score_gemma":0.00016647886,"threshold_uncertainty_score":0.005112648},"labels":[],"label_agreement":null},{"id":"W4412997328","doi":"10.3847/1538-4357/ade7fc","title":"ALMASOP. A Rotating Feature Rich in Complex Organic Molecules in a Protostellar Core","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; Herzberg Institute of Astrophysics","funders":"Ministry of Science and ICT, South Korea","keywords":"Physics; Core (optical fiber); Astrophysics; Astrochemistry; Astronomy; Feature (linguistics); Protostar; Astrobiology; Molecular cloud; Organic molecules; Stars; Molecule; Interstellar medium; Star formation; Optics; Galaxy; Quantum mechanics","score_opus":0.013289894308511397,"score_gpt":0.26279238526071425,"score_spread":0.24950249095220284,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412997328","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99846303,0.00008281598,0.00028401057,0.000012664997,0.0000032747732,0.0000042055976,0.00020005157,0.00004068393,0.00090919965],"genre_scores_gemma":[0.9992113,0.000015276502,0.0003217542,0.0000092904065,0.0000032545283,0.0000013011095,0.00019533122,0.0000039691304,0.00023858214],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999865,5.9112955e-7,4.288138e-7,0.0000052745427,0.0000025023046,0.0000046462387],"domain_scores_gemma":[0.99995303,0.000003946868,0.000016763977,0.000004299843,0.000004663142,0.000017281516],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000026703729,0.00013591861,0.00007493564,0.00046364212,0.00017297469,0.00020094686,0.00010276947,0.0001373583,0.0012671755],"category_scores_gemma":[0.000040092244,0.00005676212,0.00009005305,0.00021311278,0.00014130946,0.0000945733,0.00016979306,0.000083534986,0.00018364935],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003262376,0.00004518663,0.08619082,0.000046245143,0.00002838357,0.002014937,0.00007627007,0.0004479611,0.90039015,0.00028925965,0.000323881,0.009820728],"study_design_scores_gemma":[0.000016520245,0.00014568551,0.9452991,0.0000036907202,0.000019159652,0.0013207635,0.0000936926,0.0032850392,0.04732199,0.0002037745,0.0022842837,0.0000062778336],"about_ca_topic_score_codex":0.0013952391,"about_ca_topic_score_gemma":0.0011443577,"teacher_disagreement_score":0.0013952391,"about_ca_system_score_codex":0.00013621442,"about_ca_system_score_gemma":0.000048275244,"threshold_uncertainty_score":0.0042390823},"labels":[],"label_agreement":null},{"id":"W4412997350","doi":"10.3847/1538-4357/ade989","title":"The Connection between Galaxy Mergers, Star Formation, and Active Galactic Nuclei Activity in the HSC-SSP","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Physics; Astrophysics; Galaxy merger; Astronomy; Connection (principal bundle); Galaxy; Active galactic nucleus; Star (game theory); Star formation","score_opus":0.008128509114906911,"score_gpt":0.2281240331969199,"score_spread":0.21999552408201298,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4412997350","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99902844,0.000018929057,0.00039550333,0.000017638422,8.267729e-7,0.0000013478194,0.00027100413,0.000039050752,0.00022720295],"genre_scores_gemma":[0.9986833,0.0000090305575,0.00045205074,0.000008321212,0.0000013810521,0.0000017423887,0.000711735,0.000008311488,0.00012417723],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991417,0.000012368828,0.000003977768,0.000032173786,0.000019233403,0.000018208222],"domain_scores_gemma":[0.99962676,0.00006945201,0.00011037982,0.000040814644,0.000054645512,0.000097919874],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00023524415,0.00018062102,0.00012720231,0.0005658967,0.0001493151,0.00030749995,0.00017278775,0.00017299448,0.00092947873],"category_scores_gemma":[0.00066370366,0.00011760041,0.0001822378,0.00031742163,0.0003211823,0.00022128849,0.0004351392,0.00024866287,0.000107385604],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005042848,0.00010889514,0.9365236,0.000026907848,0.000118517215,0.00018426833,0.00025239392,0.008595125,0.03771761,0.0008871232,0.0010220805,0.014059117],"study_design_scores_gemma":[0.0000054318966,0.000050546303,0.9776564,0.0000038779203,0.000015387637,0.00008509859,0.000113110145,0.018921519,0.002481815,0.000337047,0.00032405168,0.00000568718],"about_ca_topic_score_codex":0.009006718,"about_ca_topic_score_gemma":0.012682891,"teacher_disagreement_score":0.009006718,"about_ca_system_score_codex":0.00023836643,"about_ca_system_score_gemma":0.00011112148,"threshold_uncertainty_score":0.017908573},"labels":[],"label_agreement":null},{"id":"W4413003858","doi":"10.3847/1538-4357/ade716","title":"Timing and Spectral Evolution of the Magnetar 1E 1841-045 in Outburst","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Physics; Magnetar; Astrophysics; Astronomy; Neutron star","score_opus":0.007620075633456917,"score_gpt":0.28994717125266983,"score_spread":0.28232709561921293,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413003858","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.998259,0.00012916802,0.0001396325,0.000030661668,0.0000083030145,0.000005509232,0.0003401737,0.000027422706,0.0010600387],"genre_scores_gemma":[0.99778736,0.000057089794,0.00023939049,0.000028420067,0.000015888301,0.000007061413,0.0012583396,0.000010968453,0.0005954409],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999874,0.000013472651,0.0000075428993,0.000042449556,0.000030582443,0.000031967822],"domain_scores_gemma":[0.9995395,0.000051194515,0.00018539418,0.000034372995,0.000077848206,0.00011179181],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002769476,0.00021505397,0.00036583075,0.001093055,0.00039373204,0.00046318336,0.00024175638,0.00031027486,0.00090734777],"category_scores_gemma":[0.00049101486,0.00017298754,0.00017394355,0.00045623694,0.00020957756,0.00019195442,0.00055812445,0.0003029214,0.00030976208],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005960796,0.00010499118,0.9338877,0.000076110104,0.0000580333,0.00083692383,0.00064386084,0.00047117012,0.049718495,0.00014199104,0.0009122528,0.012552434],"study_design_scores_gemma":[0.0000018625324,0.000046974677,0.9986387,0.0000033878518,0.000005913271,0.0000980178,0.000054413114,0.000095868105,0.0005039876,0.0000072093053,0.0005413334,0.0000023885393],"about_ca_topic_score_codex":0.0030621707,"about_ca_topic_score_gemma":0.008681873,"teacher_disagreement_score":0.0030621707,"about_ca_system_score_codex":0.00039606835,"about_ca_system_score_gemma":0.000090717236,"threshold_uncertainty_score":0.006088674},"labels":[],"label_agreement":null},{"id":"W4413017398","doi":"10.3847/1538-4357/ade99d","title":"A Framework for Modeling the Evolution of Young Stellar Objects","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"National Science Foundation","keywords":"Physics; Stellar evolution; Young stellar object; Stellar physics; Astrophysics; Astronomy; Stars; Star formation","score_opus":0.012551853260508995,"score_gpt":0.2634535799271743,"score_spread":0.25090172666666527,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413017398","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.059934363,0.0005926899,0.9288267,0.00079612044,0.00005022048,0.000086223816,0.0008631609,0.0003554593,0.00849505],"genre_scores_gemma":[0.672841,0.0009563732,0.31554803,0.00017042374,0.00016939608,0.00040652213,0.0011784284,0.00022161599,0.008508102],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99949396,0.00018287243,0.000026240385,0.00013686498,0.00010618076,0.00005396479],"domain_scores_gemma":[0.99853504,0.0007486255,0.00023703363,0.00012589578,0.00022327981,0.0001301029],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0018843783,0.0006582494,0.00056476647,0.0015953409,0.0011616284,0.0024713108,0.0025592404,0.0011955537,0.0031143466],"category_scores_gemma":[0.0045570135,0.00051532977,0.0014083795,0.0009205925,0.0012094105,0.0018100637,0.0015349552,0.0011645843,0.0006132793],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000012226153,0.000019328088,0.003336365,0.000021137132,0.00002711319,0.00005874488,0.00010362392,0.8651831,0.00040077083,0.1259636,0.0005538837,0.0043200133],"study_design_scores_gemma":[0.0000023430978,0.0000047649637,0.00024052257,0.0000060924935,0.0000037960626,0.000012568502,0.000014027301,0.9643488,0.00003651451,0.03443265,0.0008924072,0.000005528303],"about_ca_topic_score_codex":0.024622515,"about_ca_topic_score_gemma":0.0146503635,"teacher_disagreement_score":0.024622515,"about_ca_system_score_codex":0.0021772627,"about_ca_system_score_gemma":0.0014155115,"threshold_uncertainty_score":0.04895836},"labels":[],"label_agreement":null},{"id":"W4413025655","doi":"10.3847/1538-4357/ade9a0","title":"Are Gas-rich Ultra-diffuse Galaxies and Field Dwarfs Distinct?","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; Arthur B. McDonald-Canadian Astroparticle Physics Research Institute; University of Toronto; Queen's University","funders":"Gauss Centre for Supercomputing; Leibniz-Rechenzentrum; Natural Sciences and Engineering Research Council of Canada; Tamkeen; Ministerio de Ciencia e Innovación; York University; New York University Abu Dhabi; Leibniz-Gemeinschaft; Canada First Research Excellence Fund; National Science Foundation","keywords":"Physics; Astrophysics; Galaxy; Astronomy","score_opus":0.006328191525611252,"score_gpt":0.21531487197473184,"score_spread":0.20898668044912058,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413025655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99958426,0.000047205933,0.00011301555,0.000012913152,5.4402284e-7,9.230977e-7,0.000032978445,0.000002748176,0.00020539397],"genre_scores_gemma":[0.9998815,0.000012006078,0.00004261057,0.0000049126456,8.7848855e-7,3.0735703e-7,0.000035843423,6.138057e-7,0.000021303771],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99981743,0.000040070667,0.000007704514,0.000072829665,0.000027670902,0.000034268305],"domain_scores_gemma":[0.9991769,0.00024457625,0.0002431103,0.000106737774,0.000050641025,0.00017798327],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005604348,0.0001053551,0.00028834352,0.00052103004,0.00018773011,0.00068437937,0.0003666315,0.00020326972,0.0006919829],"category_scores_gemma":[0.0015292044,0.000112100075,0.00016284258,0.00039897554,0.0007898615,0.0005700429,0.0003928727,0.00012370913,0.00008577787],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016812044,0.000017011314,0.9907575,0.000017923563,0.000041958105,0.000047380498,0.00027566613,0.00065417925,0.0031078758,0.0007148939,0.000055386023,0.004142009],"study_design_scores_gemma":[0.000006643548,0.000025355554,0.9966365,0.0000045062334,0.00001217946,0.0000686585,0.00044585174,0.0018253309,0.00031763874,0.00047803269,0.00017581084,0.0000033422746],"about_ca_topic_score_codex":0.0045984513,"about_ca_topic_score_gemma":0.007542385,"teacher_disagreement_score":0.0045984513,"about_ca_system_score_codex":0.00035094007,"about_ca_system_score_gemma":0.00016828618,"threshold_uncertainty_score":0.0091433525},"labels":[],"label_agreement":null},{"id":"W4413036142","doi":"10.3847/1538-4357/adeb73","title":"Sleeping Giants Arise: Monitoring the Return of Three Changing-look Quasars to Their High States<sup>*</sup>","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University","funders":"","keywords":"Physics; Quasar; Astronomy; Astrophysics; Galaxy","score_opus":0.015272465500749816,"score_gpt":0.24315626905800145,"score_spread":0.22788380355725163,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413036142","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99935347,0.000022563197,0.00012652203,0.000036906,0.0000029526955,0.000009860845,0.00013513373,0.0000134919,0.000299107],"genre_scores_gemma":[0.99928504,0.000015632517,0.00027759475,0.000047855032,0.0000056471254,0.000007253625,0.0002241369,0.000004211654,0.00013275974],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999137,0.000011779136,0.0000054363286,0.00002080975,0.000020817311,0.000027383028],"domain_scores_gemma":[0.99930143,0.000088259876,0.00017891769,0.000033253018,0.000120133176,0.0002780752],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000305753,0.00014968346,0.00023438019,0.00053011905,0.0004866878,0.000409465,0.0003127455,0.00049999595,0.0007882325],"category_scores_gemma":[0.00070899475,0.00010364685,0.00014731415,0.00029954923,0.00028691234,0.00021477998,0.0005307933,0.0005792254,0.00021186395],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002921703,0.00019003743,0.97380877,0.000013482877,0.000050242903,0.0009267111,0.00095770595,0.000112144444,0.016869912,0.000115485906,0.00050439,0.006158902],"study_design_scores_gemma":[0.0000072728344,0.00015676675,0.99745625,0.0000019816114,0.00000971716,0.00041466937,0.00046630134,0.00038890573,0.00072048465,0.000056332734,0.00031532743,0.0000059224685],"about_ca_topic_score_codex":0.003186154,"about_ca_topic_score_gemma":0.009215093,"teacher_disagreement_score":0.003186154,"about_ca_system_score_codex":0.00024397748,"about_ca_system_score_gemma":0.00009469313,"threshold_uncertainty_score":0.0063352585},"labels":[],"label_agreement":null},{"id":"W4413058551","doi":"10.3847/1538-4357/addd05","title":"IceCube Search for Neutrino Emission from X-Ray Bright Seyfert Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":25,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Experimental Program to Stimulate Competitive Research; Japan Society for the Promotion of Science; Deutsches Elektronen-Synchrotron; Natural Sciences and Engineering Research Council of Canada; Office of Polar Programs; College of Engineering, Michigan State University; Helmholtz Alliance for Astroparticle Physics; Institute for Global Prominent Research, Chiba University; RWTH Aachen University; Alliance de recherche numérique du Canada; Chiba University; Knut och Alice Wallenbergs Stiftelse; Villum Fonden; National Research Foundation of Korea; Marsden Fund; Bundesministerium für Bildung und Forschung; Schweizerischer Nationalfonds zur Förderung der Wissenschaftlichen Forschung; National Science Foundation; Belgian Federal Science Policy Office; Deutsche Forschungsgemeinschaft; Michigan State University; National Research Foundation; University of Wisconsin-Madison; Vetenskapsrådet; U.S. Department of Energy; Office of Advanced Cyberinfrastructure; European Commission; Western Canada Research Grid; Fonds De La Recherche Scientifique - FNRS; Polarforskningssekretariatet; Fonds Wetenschappelijk Onderzoek; Nvidia; Marquette University","keywords":"Physics; Astrophysics; Galaxy; Neutrino; Active galactic nucleus; Astronomy; Supermassive black hole; Flux (metallurgy)","score_opus":0.009700677512185363,"score_gpt":0.24840240897674148,"score_spread":0.23870173146455612,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413058551","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99459994,0.000096594544,0.00024305715,0.000039521226,0.0000045643806,0.000013369661,0.0038152186,0.0000488299,0.0011389524],"genre_scores_gemma":[0.979159,0.00014579075,0.0014982616,0.000040115407,0.000025171159,0.000032031538,0.018515095,0.000014134506,0.0005703379],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99979156,0.000024653054,0.000010551046,0.00007914387,0.00005427178,0.00003976417],"domain_scores_gemma":[0.99924123,0.00014238329,0.00032359295,0.00006955977,0.00007979593,0.00014340246],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005932231,0.00031542368,0.00033214322,0.0013529686,0.0003306778,0.0006704275,0.00024222615,0.00029377476,0.0017576546],"category_scores_gemma":[0.0006528684,0.00012417005,0.00025033636,0.0011478061,0.00014805826,0.0002165141,0.00048899546,0.00017989158,0.00029346126],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031059774,0.000087563174,0.9818965,0.000024814604,0.000116504256,0.0001813699,0.00007388376,0.0008306527,0.0077789775,0.0001610991,0.0013865649,0.0071514435],"study_design_scores_gemma":[0.000024898723,0.00008811946,0.99396884,0.000008806692,0.00004534613,0.00015930571,0.000094955205,0.0018992979,0.0019440575,0.00008621472,0.001676505,0.000003639342],"about_ca_topic_score_codex":0.0044653052,"about_ca_topic_score_gemma":0.008481681,"teacher_disagreement_score":0.0044653052,"about_ca_system_score_codex":0.00033146216,"about_ca_system_score_gemma":0.00025209176,"threshold_uncertainty_score":0.008878648},"labels":[],"label_agreement":null},{"id":"W4413084389","doi":"10.3847/1538-4357/ade2e6","title":"Comprehensive Radio Monitoring of the Black Hole X-Ray Binary Swift J1727.8−1613 during Its 2023–2024 Outburst","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Smithsonian Astrophysical Observatory; University of Cape Town; European Commission; INAF - Osservatorio Astrofisico di Catania; National Astronomical Observatory of Japan; RIKEN; Korea Astronomy and Space Science Institute; National Institutes of Natural Sciences; HORIZON EUROPE Framework Programme; University of the Western Cape; Canada Research Chairs; Australian Government; Japan Aerospace Exploration Agency; Commonwealth Scientific and Industrial Research Organisation; Academia Sinica; National Science Foundation; UK Research and Innovation; National Research Foundation; University of Pretoria; University of Warwick; Smithsonian Institution; National Radio Astronomy Observatory; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Astrophysics; Light curve; Swift; Astronomy; Black hole (networking); Radiative transfer","score_opus":0.014978314412876744,"score_gpt":0.24711391510133401,"score_spread":0.23213560068845726,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413084389","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984006,0.00010638574,0.00014104054,0.000027254015,0.0000065510017,0.000009991695,0.00045226686,0.000011795976,0.00084409607],"genre_scores_gemma":[0.99576193,0.00011445942,0.0004908149,0.00003307755,0.000028484357,0.000014020644,0.00276705,0.000011446853,0.00077877735],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998542,0.00001096107,0.000008532566,0.00003240718,0.000048666294,0.000045183187],"domain_scores_gemma":[0.9995235,0.000027070324,0.00012577488,0.0000325187,0.00014648544,0.00014464662],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042707822,0.0001540966,0.00023668466,0.0010180401,0.0005413239,0.00043979558,0.00020615537,0.00016698649,0.00056519],"category_scores_gemma":[0.00029439945,0.0000804137,0.00012286447,0.0005456663,0.0001865405,0.00022712024,0.0006527829,0.00021475871,0.00031153669],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030162567,0.00013986089,0.9234849,0.000052792184,0.00005572245,0.0009370967,0.0008801677,0.00047539576,0.035396967,0.00022743118,0.0019386407,0.036109492],"study_design_scores_gemma":[0.0000052362743,0.00007453238,0.9956251,0.0000064734145,0.000011597811,0.00014892928,0.0001935983,0.00027749958,0.0012543233,0.000026346333,0.002371791,0.000004667341],"about_ca_topic_score_codex":0.009151103,"about_ca_topic_score_gemma":0.024908563,"teacher_disagreement_score":0.009151103,"about_ca_system_score_codex":0.00038591825,"about_ca_system_score_gemma":0.00033513058,"threshold_uncertainty_score":0.018195689},"labels":[],"label_agreement":null},{"id":"W4413093339","doi":"10.3847/1538-4357/ade4ce","title":"C-19 and Hot, Wide Star Streams","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"National Science and Technology Council; Science and Technology Facilities Council; National Tsing Hua University; Villum Fonden; University of Toronto; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Durham University; Government of Ontario","keywords":"Physics; Globular cluster; Milky Way; Astrophysics; Galactic halo; Velocity dispersion; Astronomy; Star cluster; Population; Dark matter halo; Halo; Galaxy","score_opus":0.0070009938586833,"score_gpt":0.22429896798143098,"score_spread":0.21729797412274768,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413093339","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99640524,0.000020872483,0.0004361313,0.000039191375,0.000004543099,0.0000073061583,0.00005649836,0.000012594484,0.0030177527],"genre_scores_gemma":[0.9980842,0.00002380662,0.00031440405,0.000015612495,0.000005164683,0.0000040982436,0.00012218417,0.0000073491237,0.001423237],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.9999541,0.000007612716,0.0000016209646,0.00001051831,0.00000838852,0.000017749115],"domain_scores_gemma":[0.99967253,0.000057142097,0.000056645746,0.0000151442955,0.000029423543,0.00016917958],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013876389,0.00024710916,0.00024298485,0.00024765494,0.0005122867,0.0008705773,0.0004109398,0.00047977103,0.0028353164],"category_scores_gemma":[0.0006699871,0.00011769363,0.00021723144,0.00022894893,0.00057684234,0.00057867414,0.00078425027,0.00032990603,0.00022269857],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0015047471,0.0005326705,0.25484985,0.00007016444,0.00013093451,0.005758068,0.0005290452,0.5907245,0.017341023,0.11597402,0.0032114773,0.009373447],"study_design_scores_gemma":[0.00047802855,0.00049083156,0.063734785,0.000026478843,0.000072341,0.00097510894,0.00068194885,0.89524186,0.005520076,0.026762115,0.005963766,0.000052602652],"about_ca_topic_score_codex":0.008205777,"about_ca_topic_score_gemma":0.0057643577,"teacher_disagreement_score":0.008205777,"about_ca_system_score_codex":0.0008023599,"about_ca_system_score_gemma":0.00043465392,"threshold_uncertainty_score":0.016315997},"labels":[],"label_agreement":null},{"id":"W4413131707","doi":"10.3847/1538-4357/ade686","title":"Planetary Obliquity Excitation through Pre-main-sequence Stellar Evolution","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Massachusetts Green High Performance Computing Center","keywords":"Physics; Planet; Astrophysics; Exoplanet; Astronomy; Planetary system; Adiabatic process; Quantum mechanics","score_opus":0.015058868160502791,"score_gpt":0.25918365085107015,"score_spread":0.24412478269056737,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413131707","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984856,0.00006701762,0.00021738347,0.00001920098,0.0000015885953,0.0000013535505,0.000028727432,0.00001424587,0.0011649767],"genre_scores_gemma":[0.99975437,0.000019688618,0.000042997577,0.000004318421,5.2871934e-7,5.399506e-7,0.000021019114,0.00000288558,0.00015375866],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9999628,0.000004853602,0.0000014613169,0.000011760003,0.000007378309,0.000011768486],"domain_scores_gemma":[0.9998661,0.000025683823,0.000041618172,0.000013105384,0.000022324177,0.00003116611],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010025789,0.00012303329,0.0001027243,0.0001837744,0.00023675803,0.0003447812,0.000118460615,0.00018985585,0.001387939],"category_scores_gemma":[0.00040436312,0.00009974381,0.000107190404,0.00011936478,0.00025886486,0.00020446186,0.0003036472,0.00018280446,0.00019922815],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003568417,0.000084823514,0.6604161,0.00008033196,0.0000998865,0.00081513525,0.000637546,0.009185247,0.3064729,0.0027474987,0.0004885979,0.01861514],"study_design_scores_gemma":[0.0000060961997,0.00008705285,0.9747376,0.000009537248,0.000015299356,0.00028477403,0.00023179714,0.009669952,0.012902156,0.0006684995,0.0013778294,0.000009392924],"about_ca_topic_score_codex":0.0022102536,"about_ca_topic_score_gemma":0.002755347,"teacher_disagreement_score":0.0022102536,"about_ca_system_score_codex":0.00035147395,"about_ca_system_score_gemma":0.00012554182,"threshold_uncertainty_score":0.004643142},"labels":[],"label_agreement":null},{"id":"W4413141863","doi":"10.3847/1538-4357/adf0fa","title":"Multiwavelength Constraints on Dust Dynamics and Size Evolution in Protoplanetary Disk Rings. I. Method","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Science and Technology Council; National Natural Science Foundation of China; Natural Science Foundation of Shanghai","keywords":"Physics; Protoplanetary disk; Astrophysics; Dynamics (music); Astronomy; Accretion disc; Planet","score_opus":0.0059397609337843325,"score_gpt":0.2532147121515219,"score_spread":0.24727495121773757,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413141863","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.58125705,0.0005294103,0.3995429,0.00042448638,0.000059917464,0.00037892445,0.0046206675,0.0012734799,0.011913177],"genre_scores_gemma":[0.88848555,0.0002100394,0.107845925,0.00010691597,0.000035535602,0.0003509339,0.00096228416,0.00016396448,0.0018387948],"study_design_codex":"simulation_or_modeling","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.99980575,0.000060476326,0.000012106713,0.00006074181,0.00003334152,0.000027479004],"domain_scores_gemma":[0.9992888,0.00028156556,0.00015306615,0.00015264485,0.00006286365,0.0000609447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005109814,0.0004034348,0.00044019296,0.0005224409,0.00048704352,0.00078125513,0.0019961845,0.00090731616,0.0025467507],"category_scores_gemma":[0.002083296,0.00046251694,0.0006967192,0.00044462844,0.0004042427,0.0007413572,0.00067278487,0.00042441484,0.00038379253],"study_design_candidate":"bench_or_experimental","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015582013,0.00026021453,0.0573708,0.00020841336,0.0001420589,0.00042836546,0.00012553355,0.87752974,0.011758243,0.025884964,0.0012933617,0.024842475],"study_design_scores_gemma":[0.000044218756,0.000015706608,0.00413348,0.000010328138,0.000010887071,0.000080332786,0.000022254677,0.98876077,0.0016857812,0.00407655,0.0011306667,0.000029014971],"about_ca_topic_score_codex":0.006376032,"about_ca_topic_score_gemma":0.0036985292,"teacher_disagreement_score":0.006376032,"about_ca_system_score_codex":0.00070004934,"about_ca_system_score_gemma":0.00070814934,"threshold_uncertainty_score":0.012677848},"labels":[],"label_agreement":null},{"id":"W4413168937","doi":"10.3847/1538-4357/adef2f","title":"Rotation Signatures of TESS B-type Stars: Enlarging the Sample","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Montreal Clinical Research Institute","funders":"Coordenação de Aperfeiçoamento de Pessoal de Nível Superior","keywords":"Physics; Stars; Astrophysics; Astronomy; Rotation (mathematics); Geometry","score_opus":0.009404970961325584,"score_gpt":0.24295652860828051,"score_spread":0.23355155764695493,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413168937","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99864393,0.000056621415,0.00067886827,0.000008918871,0.0000017208491,0.0000062034965,0.00020117461,0.000016694437,0.00038591833],"genre_scores_gemma":[0.9954358,0.00008826071,0.0025391572,0.000011951875,0.00001750981,0.000011499379,0.001714635,0.000010666186,0.00017048769],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977106,0.000052946943,0.000022593927,0.000065503504,0.000049078117,0.00003874479],"domain_scores_gemma":[0.9992471,0.0001514291,0.00014078019,0.00017073244,0.00013743066,0.00015252687],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005978337,0.00017498125,0.0003334253,0.0026363088,0.00033871812,0.00034327136,0.00019144152,0.00016550942,0.0011563303],"category_scores_gemma":[0.0008735433,0.00009929286,0.00031002148,0.0013371424,0.00017759184,0.00030164185,0.00068964076,0.00020304522,0.00047708358],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002890058,0.000085151296,0.9157628,0.000032964843,0.000040562147,0.00013976608,0.00023563011,0.0005784751,0.032326702,0.00013712919,0.0003532088,0.050018724],"study_design_scores_gemma":[0.0000058362225,0.00009149932,0.99425656,0.000005218545,0.000012198315,0.00023564333,0.00013263877,0.0021206292,0.0016566737,0.00008511839,0.001394259,0.0000037275136],"about_ca_topic_score_codex":0.0014075126,"about_ca_topic_score_gemma":0.002190166,"teacher_disagreement_score":0.0026363088,"about_ca_system_score_codex":0.00013109541,"about_ca_system_score_gemma":0.00016051276,"threshold_uncertainty_score":0.0038682818},"labels":[],"label_agreement":null},{"id":"W4413174050","doi":"10.3847/1538-4357/aded13","title":"AT 2019aalc: A Bowen Fluorescence Flare with a Precursor Flare in an Active Galactic Nucleus","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Advanced Research","funders":"Israel Science Foundation; Narodowe Centrum Nauki; Deutsche Forschungsgemeinschaft; UK Research and Innovation","keywords":"Physics; Flare; Active galactic nucleus; Astrophysics; Nucleus; Astronomy; Solar flare; Galaxy","score_opus":0.008834930527641722,"score_gpt":0.24099563271643878,"score_spread":0.23216070218879706,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413174050","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9968514,0.00007701467,0.00016717472,0.000049483526,0.000019182831,0.000023026467,0.00091622316,0.00004559171,0.0018509798],"genre_scores_gemma":[0.9971545,0.000017208647,0.0002534287,0.0000392272,0.000017586639,0.000007819468,0.0020435464,0.0000066729463,0.00046005036],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982053,0.0000061824517,0.00000866971,0.000040456653,0.000050695107,0.000073475756],"domain_scores_gemma":[0.99960357,0.000019271414,0.000099265235,0.00003265491,0.000084653715,0.00016068728],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014373384,0.0002469829,0.00031501285,0.0010858605,0.00091318216,0.0006353929,0.0002665668,0.0005085214,0.0013062466],"category_scores_gemma":[0.0003155241,0.00009230576,0.00028134548,0.00073595677,0.00022424142,0.00023288412,0.00060578325,0.00036062664,0.00031796136],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0008477483,0.00042870443,0.9119145,0.00007609773,0.00015437217,0.006528629,0.00035626328,0.0008488085,0.05389746,0.0005177079,0.0040726685,0.020356985],"study_design_scores_gemma":[0.000010841719,0.00011676796,0.9944924,0.000008511743,0.000014681215,0.000955366,0.00013523402,0.00049560546,0.001794804,0.00006449253,0.001899733,0.000011530454],"about_ca_topic_score_codex":0.018772546,"about_ca_topic_score_gemma":0.03354079,"teacher_disagreement_score":0.018772546,"about_ca_system_score_codex":0.0009942547,"about_ca_system_score_gemma":0.00027860995,"threshold_uncertainty_score":0.037326574},"labels":[],"label_agreement":null},{"id":"W4413202290","doi":"10.3847/1538-4357/aded90","title":"Cold Gas and Star Formation in the Phoenix Cluster with JWST","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Université de Montréal","funders":"Smithsonian Astrophysical Observatory; National Aeronautics and Space Administration; Space Telescope Science Institute; Smithsonian Institution; National Science Foundation","keywords":"Physics","score_opus":0.006247389676372386,"score_gpt":0.22265201947206892,"score_spread":0.21640462979569652,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413202290","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9966196,0.000032656626,0.00029338515,0.00006505295,0.0000033753513,0.000006716632,0.0012197853,0.00009440636,0.0016650625],"genre_scores_gemma":[0.99494654,0.00003856621,0.0010396455,0.00004272034,0.000011937301,0.0000063404086,0.0028547493,0.000043108736,0.0010164599],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998629,0.000009006921,0.000004052009,0.000063083586,0.000031159238,0.000029878225],"domain_scores_gemma":[0.999724,0.000022871063,0.000061146166,0.000050444938,0.00004407992,0.00009750046],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0002611273,0.0002469125,0.00016883554,0.00046567823,0.00030549278,0.00045314335,0.00037987367,0.00017570285,0.0020469187],"category_scores_gemma":[0.00043454106,0.00013472413,0.00012234457,0.00049734284,0.00021369064,0.00042619059,0.0006691582,0.0003363879,0.00038996988],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004777624,0.00015454389,0.93996304,0.000033262073,0.00013819471,0.00042445314,0.00048084487,0.0051911166,0.032244507,0.00058662187,0.006535094,0.013770518],"study_design_scores_gemma":[0.000016621525,0.000030152798,0.99077153,0.0000037120012,0.000012900564,0.00006852317,0.00008924296,0.00374489,0.0028347254,0.000072704526,0.0023487348,0.0000062331433],"about_ca_topic_score_codex":0.025338275,"about_ca_topic_score_gemma":0.025939334,"teacher_disagreement_score":0.025338275,"about_ca_system_score_codex":0.0005202038,"about_ca_system_score_gemma":0.00015579745,"threshold_uncertainty_score":0.05038154},"labels":[],"label_agreement":null},{"id":"W4413217648","doi":"10.3847/1538-4357/adea51","title":"Metallicity Gradients in Modern Cosmological Simulations. I. Tension between Smooth Stellar Feedback Models and Observations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":12,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"Virginia Space Grant Consortium","keywords":"Physics; Astrophysics; Metallicity; Redshift; Galaxy; Stellar mass; Star formation; Galaxy formation and evolution; Astronomy","score_opus":0.031593298233653234,"score_gpt":0.24652553394668641,"score_spread":0.2149322357130332,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413217648","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99725926,0.000045865974,0.00084423576,0.00013775266,0.0000061715205,0.000006637437,0.00024026437,0.000098397075,0.0013613903],"genre_scores_gemma":[0.9983828,0.000024956304,0.00094282744,0.000053455064,0.000004251383,0.000008536261,0.00029890458,0.000035402198,0.00024888673],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983156,0.000055805773,0.00001128712,0.000035906534,0.000028836032,0.000036538757],"domain_scores_gemma":[0.9991726,0.00034995432,0.00013836344,0.00012333826,0.00010283258,0.000112875634],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0006789374,0.0003679549,0.00032265054,0.00039252324,0.00033497342,0.0005911331,0.00075602497,0.00055358827,0.0009423839],"category_scores_gemma":[0.0040054643,0.00024842494,0.00042390314,0.0003084245,0.00047847422,0.0006251896,0.00044730562,0.00050928,0.00012779694],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031917056,0.0002126623,0.16527142,0.00006218929,0.00022623842,0.00017177072,0.0002560575,0.81719947,0.005441554,0.0045306557,0.0012400189,0.0050687618],"study_design_scores_gemma":[0.000075988086,0.0000874675,0.0214123,0.000010417027,0.00003495693,0.000032002263,0.00009442099,0.9751567,0.0013918135,0.0010918196,0.000592989,0.00001910257],"about_ca_topic_score_codex":0.021806063,"about_ca_topic_score_gemma":0.018613676,"teacher_disagreement_score":0.021806063,"about_ca_system_score_codex":0.00076849974,"about_ca_system_score_gemma":0.00040720904,"threshold_uncertainty_score":0.043358266},"labels":[],"label_agreement":null},{"id":"W4413229446","doi":"10.3847/1538-4357/aded17","title":"Constraining the Faint-end Slope of the Fast Radio Burst Energy Function Using CHIME/FRB Catalog-1 and Local Volume Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"","keywords":"Physics; Magnetar; Astrophysics; Galaxy; Population; Astronomy; Fast radio burst; Pulsar","score_opus":0.009027775823917613,"score_gpt":0.2648081552111122,"score_spread":0.25578037938719456,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413229446","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99521184,0.00013052262,0.0016675253,0.00002255845,0.0000024298758,0.00000743308,0.0017226532,0.00010835226,0.0011266937],"genre_scores_gemma":[0.99447167,0.000028902898,0.0011701706,0.00001570231,0.000004130792,0.0000066178163,0.0040737432,0.000018234447,0.00021084044],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99970955,0.000035607576,0.000014629566,0.000118195596,0.000058931968,0.00006292425],"domain_scores_gemma":[0.9980868,0.00042618645,0.00061623513,0.0004053724,0.00017996476,0.0002854513],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007603597,0.0002941175,0.00022821187,0.0026158842,0.00027994075,0.00093484455,0.00032202824,0.00025429795,0.0019020215],"category_scores_gemma":[0.0027508382,0.0001672464,0.00021562682,0.0012913635,0.00019076242,0.00037735075,0.0006296962,0.00019618263,0.0006390909],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000037648922,0.000013204045,0.9895588,0.000014541373,0.00004377033,0.000037745842,0.000071309565,0.0007173037,0.0035424903,0.00016692044,0.00033458765,0.0054618213],"study_design_scores_gemma":[0.0000029336695,0.000008118665,0.996555,0.00000851484,0.000014127374,0.00004088086,0.00006954678,0.002030449,0.00053037354,0.00008080473,0.0006555732,0.000003863546],"about_ca_topic_score_codex":0.011624006,"about_ca_topic_score_gemma":0.01496405,"teacher_disagreement_score":0.011624006,"about_ca_system_score_codex":0.0003072069,"about_ca_system_score_gemma":0.00021629046,"threshold_uncertainty_score":0.023112714},"labels":[],"label_agreement":null},{"id":"W4413229460","doi":"10.3847/1538-4357/adec7a","title":"A First Look at Spatially Resolved Infrared Supernova Remnants in M33 with JWST","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Physics; Astrophysics; Ejecta; Supernova; Astronomy; James Webb Space Telescope; Infrared; Star formation; Galaxy","score_opus":0.006430645131910404,"score_gpt":0.21011164164280016,"score_spread":0.20368099651088975,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413229460","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99914014,0.00011053841,0.00010938675,0.000011966872,0.0000011420628,0.0000041354906,0.00010169571,0.000012544883,0.00050831545],"genre_scores_gemma":[0.99920374,0.00005490237,0.0002621852,0.000015880021,0.0000056874915,0.0000021811065,0.00027741495,0.000004945055,0.00017312601],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999372,0.000005501726,0.0000054813636,0.000012829304,0.000015212134,0.000023780933],"domain_scores_gemma":[0.99967873,0.000027550606,0.00012279204,0.000034604018,0.000043542343,0.000092927716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016182006,0.00023393544,0.00018511027,0.0011770328,0.0003241437,0.00040515297,0.00014565299,0.00020856784,0.0016463663],"category_scores_gemma":[0.00034619632,0.00013753747,0.00024125418,0.00064985646,0.00024413271,0.00024829566,0.0006461577,0.00018337707,0.00031866328],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00021519096,0.000040403585,0.94871736,0.00003456119,0.0000540933,0.0026200705,0.0008700353,0.00013197938,0.039498247,0.00010990439,0.00031453365,0.0073935795],"study_design_scores_gemma":[0.0000021843332,0.000060239843,0.99705076,0.000006096507,0.000016057269,0.0009062613,0.00023185459,0.000098189696,0.0009028668,0.000022696682,0.000699665,0.0000029289438],"about_ca_topic_score_codex":0.0050652316,"about_ca_topic_score_gemma":0.008476229,"teacher_disagreement_score":0.0050652316,"about_ca_system_score_codex":0.00017629894,"about_ca_system_score_gemma":0.00009125047,"threshold_uncertainty_score":0.010071516},"labels":[],"label_agreement":null},{"id":"W4413229461","doi":"10.3847/1538-4357/adf3a8","title":"A Unified Volumetric Rate–Energy Relation from Magnetar Radio Bursts to Fast Radio Bursts","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Magnetar; Physics; Millisecond; Astrophysics; Fast radio burst; Astronomy; Neutron star","score_opus":0.007880733076332023,"score_gpt":0.27559855692334684,"score_spread":0.2677178238470148,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413229461","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9754068,0.0012878824,0.014360861,0.000093321396,0.000013269102,0.000037946873,0.00058102724,0.00030150873,0.007917327],"genre_scores_gemma":[0.9985091,0.0001626801,0.00077822636,0.000015791624,0.000008107788,0.000006530741,0.00018143932,0.000011360687,0.00032668546],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99982506,0.000019967036,0.000013446397,0.00005519725,0.00004903585,0.000037380465],"domain_scores_gemma":[0.99818146,0.00063416926,0.00073383335,0.00018682088,0.00016930576,0.00009446733],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003365653,0.00027833943,0.0001664495,0.0013275349,0.00015277517,0.00073348684,0.00050042075,0.0002789007,0.0018662278],"category_scores_gemma":[0.0028015638,0.00022080436,0.00023709801,0.0005939263,0.0005287416,0.00053451554,0.0004715156,0.0003105122,0.00039770754],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024720028,0.00006738619,0.8493283,0.00014652139,0.00015094229,0.0004639107,0.00028947368,0.006409201,0.0948129,0.007186561,0.0006642423,0.040233433],"study_design_scores_gemma":[0.0000073124156,0.00006925484,0.98396,0.000011975691,0.000038817227,0.0004832419,0.000096336786,0.006175211,0.0060134465,0.0021691474,0.0009552463,0.000020012347],"about_ca_topic_score_codex":0.0028324707,"about_ca_topic_score_gemma":0.0014665003,"teacher_disagreement_score":0.0028324707,"about_ca_system_score_codex":0.0003817305,"about_ca_system_score_gemma":0.000119800716,"threshold_uncertainty_score":0.0062431097},"labels":[],"label_agreement":null},{"id":"W4413250397","doi":"10.3847/1538-4357/adee15","title":"Constraints on Fast Radio Burst Population from the First CHIME/FRB Catalog with the Hierarchical Bayesian Inference","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Physics; Redshift; Astrophysics; Cosmology; Inference; Population; Bayesian inference; Astronomy; Bayesian probability; Galaxy; Artificial intelligence; Computer science","score_opus":0.007686675489258969,"score_gpt":0.2842257199223942,"score_spread":0.27653904443313526,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413250397","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.87300533,0.0006598791,0.115903325,0.00042714967,0.000014712025,0.000095059615,0.005410149,0.00036325573,0.004121209],"genre_scores_gemma":[0.9794189,0.00011925772,0.01619005,0.00003937108,0.000015497895,0.000019499357,0.0036997488,0.00003646435,0.00046122895],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999087,0.00028483573,0.000036831927,0.00025329948,0.00018725822,0.00015085816],"domain_scores_gemma":[0.99359316,0.003749019,0.00089888327,0.00072728423,0.0006457721,0.0003858406],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003978474,0.0003599068,0.00039141718,0.002606999,0.00080560026,0.0017710078,0.0010631239,0.00047594277,0.0025547857],"category_scores_gemma":[0.014554128,0.0003061056,0.000516561,0.0019265431,0.00066397194,0.0008935563,0.00093747984,0.00060984446,0.00025814568],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023846768,0.00008910147,0.83083886,0.00012220273,0.00039323312,0.0002202756,0.00046349323,0.071434334,0.007661151,0.015451712,0.0031995173,0.06988763],"study_design_scores_gemma":[0.00003696458,0.000024977875,0.6285766,0.000042376865,0.00013475677,0.000090631795,0.00019786214,0.35679656,0.0014861358,0.00927313,0.0032849244,0.000054980555],"about_ca_topic_score_codex":0.33278227,"about_ca_topic_score_gemma":0.3433503,"teacher_disagreement_score":0.33278227,"about_ca_system_score_codex":0.0022986117,"about_ca_system_score_gemma":0.0028124403,"threshold_uncertainty_score":0.66169053},"labels":[],"label_agreement":null},{"id":"W4413293574","doi":"10.3847/1538-4357/adf106","title":"Weak X-Ray Bursts on Slowly Accreting Neutron Stars","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; University of Washington; National Aeronautics and Space Administration; U.S. Department of Energy; National Science Foundation","keywords":"Physics; Neutron star; Astrophysics; Astronomy; Stars; Accretion (finance)","score_opus":0.010082307628268044,"score_gpt":0.31460813293490325,"score_spread":0.3045258253066352,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413293574","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990096,0.000035728764,0.00017907537,0.000007259735,0.0000017385487,0.0000029937987,0.00012403917,0.000017262577,0.0006222258],"genre_scores_gemma":[0.9992137,0.000028992901,0.00025703525,0.000004170964,0.0000023515659,0.0000027589272,0.00026038475,0.0000086954815,0.00022177718],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999336,0.000007952311,0.000005623448,0.000021375094,0.000018036097,0.000013444766],"domain_scores_gemma":[0.9997296,0.000064659136,0.00009042558,0.000028699298,0.000021730119,0.0000649252],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016085105,0.00026442256,0.00020565474,0.00040908222,0.00020919702,0.00040021163,0.0002049127,0.00018905757,0.0011142318],"category_scores_gemma":[0.0004622007,0.000107503016,0.00016279165,0.00028428665,0.00017900253,0.00018792137,0.0005171263,0.0001988647,0.00020669543],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012066643,0.00009770905,0.7972759,0.000107378626,0.00009033232,0.0008503155,0.00037867815,0.012659838,0.16949116,0.0012657508,0.00034521925,0.016231108],"study_design_scores_gemma":[0.00004484733,0.0002818895,0.93716586,0.000016437725,0.000033675664,0.00040170553,0.00018858684,0.032296885,0.027100015,0.00067247165,0.0017810035,0.000016612797],"about_ca_topic_score_codex":0.001114367,"about_ca_topic_score_gemma":0.0012614261,"teacher_disagreement_score":0.001114367,"about_ca_system_score_codex":0.00027589028,"about_ca_system_score_gemma":0.000073459596,"threshold_uncertainty_score":0.003727436},"labels":[],"label_agreement":null},{"id":"W4413363665","doi":"10.3847/1538-4357/adee20","title":"Robustness of Neural Ratio and Posterior Estimators to Distributional Shifts for Population-level Dark Matter Analysis in Strong Gravitational Lensing","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Dark Matter and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Perimeter Institute; Mila - Quebec Artificial Intelligence Institute; Université de Montréal; Centre for Research in Astrophysics of Québec; Montreal Heart Institute","funders":"","keywords":"Physics; Estimator; Dark matter; Weak gravitational lensing; Gravitational lens; Robustness (evolution); Strong gravitational lensing; Astrophysics; Population; Gravitation; Statistical physics; Astronomy; Statistics; Medicine; Galaxy","score_opus":0.011975247881351125,"score_gpt":0.2676374133182446,"score_spread":0.25566216543689346,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413363665","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.6521646,0.00061831577,0.34341848,0.0007349165,0.00006131381,0.00006893506,0.00031309656,0.0006391082,0.0019811783],"genre_scores_gemma":[0.9701811,0.000099017685,0.028710397,0.000118012744,0.00003324207,0.00003110991,0.00042236847,0.000057240402,0.00034752197],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9958528,0.002586273,0.0002298657,0.00065303006,0.000529053,0.0001491113],"domain_scores_gemma":[0.9329852,0.056951955,0.002769712,0.004273369,0.0024530378,0.0005666544],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.025627831,0.0007630549,0.0007603959,0.0011500053,0.0004741955,0.0012905839,0.002004596,0.0013202337,0.0010192741],"category_scores_gemma":[0.11783876,0.0004555308,0.00058611785,0.0005207133,0.002441378,0.0024307335,0.0023913647,0.0016900967,0.00024963636],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00058034377,0.00010589678,0.05516458,0.00015260834,0.0004788957,0.0000879198,0.00014505301,0.87278724,0.003900642,0.008308107,0.00057068304,0.057718087],"study_design_scores_gemma":[0.000015791402,0.00007098109,0.007417651,0.000024509385,0.000021858012,0.000044474273,0.000037744787,0.9830026,0.0026840405,0.0064985263,0.00016096987,0.000020978889],"about_ca_topic_score_codex":0.0041890093,"about_ca_topic_score_gemma":0.0027064607,"teacher_disagreement_score":0.025627831,"about_ca_system_score_codex":0.00087267807,"about_ca_system_score_gemma":0.0007870616,"threshold_uncertainty_score":0.13553458},"labels":[],"label_agreement":null},{"id":"W4413436233","doi":"10.3847/1538-4357/aded8f","title":"Magnetic White Dwarfs in the SDSS 100 pc Sample: Further Evidence of Two Formation Channels","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":7,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal","funders":"Agencia Estatal de Investigación; Nuclear Safety and Security Commission; European Commission; Agencia Nacional de Investigación y Desarrollo; Korea Astronomy and Space Science Institute; National Aeronautics and Space Administration; Dartmouth College; Ohio State University; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Generalitat de Catalunya; Agència de Gestió d'Ajuts Universitaris i de Recerca; National Science Foundation","keywords":"Physics; White dwarf; Astrophysics; Astronomy; Massive compact halo object; Sample (material); Stars","score_opus":0.019373559283376387,"score_gpt":0.2683212809822863,"score_spread":0.2489477216989099,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413436233","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994128,0.000029174571,0.000196874,0.000031080643,0.0000010716764,0.0000020598322,0.00019608234,0.000016532578,0.00011439432],"genre_scores_gemma":[0.99914765,0.000015420876,0.00011143213,0.000010681586,0.0000047304284,0.0000023233774,0.00059799186,0.000011360907,0.000098375276],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9994099,0.000117398624,0.00003406799,0.0001835435,0.00012783326,0.0001272031],"domain_scores_gemma":[0.9980386,0.000642765,0.000502923,0.00024816394,0.00019795622,0.00036964647],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0010205081,0.00032737263,0.00054046884,0.001129797,0.0006362603,0.0012365951,0.00043546158,0.00026517012,0.0015088668],"category_scores_gemma":[0.0023925924,0.00025830817,0.0007053901,0.0009941198,0.0005152345,0.0005851491,0.0010331224,0.00034113953,0.00034985892],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000100895995,0.00002785731,0.99540776,0.0000068733243,0.000050991264,0.00006913205,0.00019530625,0.0005343981,0.0014266219,0.00016903217,0.00022085535,0.0017901896],"study_design_scores_gemma":[0.00001241417,0.000018460334,0.9929743,0.0000023404193,0.000023871502,0.000067477784,0.00019360264,0.0060097086,0.00025177348,0.00012827363,0.00031188945,0.000005719759],"about_ca_topic_score_codex":0.013528183,"about_ca_topic_score_gemma":0.009788159,"teacher_disagreement_score":0.013528183,"about_ca_system_score_codex":0.00043856475,"about_ca_system_score_gemma":0.0004759364,"threshold_uncertainty_score":0.026898861},"labels":[],"label_agreement":null},{"id":"W4413440430","doi":"10.3847/1538-4357/adef4c","title":"Production of Radioactive <sup>22</sup>Na in Core-collapse Supernovae: The Ne-E(L) Component in Presolar Grains and Its Possible Consequences on Supernova Observations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; TRIUMF","funders":"Office of International Science and Engineering; Science and Technology Facilities Council; Nuclear Physics; Natural Sciences and Engineering Research Council of Canada; Magyar Tudományos Akadémia; Nuclear Safety and Security Commission; Los Alamos National Laboratory; National Nuclear Security Administration; Office of Science; Nemzeti Kutatási Fejlesztési és Innovációs Hivatal; U.S. Department of Energy; European Commission; University of Hull; National Aeronautics and Space Administration; University of Victoria; National Science Foundation","keywords":"Physics; Supernova; Presolar grains; Nucleosynthesis; Astrophysics; Component (thermodynamics); Astronomy; Type II supernova; Stellar evolution; Stars","score_opus":0.024661478874426757,"score_gpt":0.2468818431340294,"score_spread":0.22222036425960262,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413440430","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99844676,0.00022234704,0.00061804167,0.0000063664775,0.0000018790579,0.0000040770256,0.00019037677,0.000023755114,0.00048644785],"genre_scores_gemma":[0.9993129,0.000059394788,0.00021426984,0.0000034982938,0.0000017155535,0.0000016688543,0.0002686764,0.000006193094,0.00013180151],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998822,0.000012974237,0.000010464189,0.000043996002,0.000028189443,0.000022123888],"domain_scores_gemma":[0.99969447,0.00006775646,0.000110233705,0.00003810149,0.000042809414,0.00004669476],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00038855252,0.00034192114,0.00020157803,0.0006999523,0.00020325421,0.00081147224,0.00029051738,0.00045868725,0.0008910381],"category_scores_gemma":[0.00036681784,0.00020149272,0.00032552428,0.00041063377,0.00028483305,0.0002175573,0.00031571763,0.00013358932,0.0002393514],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011837576,0.000051596824,0.6986519,0.00010114101,0.00015523803,0.000881489,0.00011309436,0.0034075412,0.28749904,0.000459988,0.00009757295,0.0073975823],"study_design_scores_gemma":[0.000018138635,0.00023240467,0.89614874,0.000012352028,0.00008501151,0.00094578566,0.00014248703,0.013247559,0.08730337,0.0003820112,0.0014597574,0.000022429602],"about_ca_topic_score_codex":0.0027973708,"about_ca_topic_score_gemma":0.0024312565,"teacher_disagreement_score":0.0027973708,"about_ca_system_score_codex":0.00032452217,"about_ca_system_score_gemma":0.0001048013,"threshold_uncertainty_score":0.0055621862},"labels":[],"label_agreement":null},{"id":"W4413488469","doi":"10.3847/1538-4357/adf32d","title":"XRISM Constrains Atmospheric Motion and Turbulent Dissipation in the Archetypal Radio-mode Feedback System Hydra-A","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo","funders":"Canadian Space Agency; Nuclear Safety and Security Commission; Grantová Agentura České Republiky; University of Nottingham; National Aeronautics and Space Administration","keywords":"Physics; Lernaean Hydra; Dissipation; Turbulence; Mode (computer interface); Astronomy; Motion (physics); Astrophysics; Classical mechanics; Mechanics; Quantum mechanics","score_opus":0.005947656522853998,"score_gpt":0.22486499972554216,"score_spread":0.21891734320268816,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413488469","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993988,0.000024325973,0.00012097454,0.000010704444,0.0000011213664,0.000001682595,0.00013101613,0.000027243514,0.000284151],"genre_scores_gemma":[0.99963033,0.000007727081,0.00017819638,0.0000066586763,0.0000017839291,0.0000013743826,0.00011609302,0.0000058694227,0.000051843064],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993193,0.0000064550563,0.0000026392545,0.00002606061,0.000010023477,0.00002295988],"domain_scores_gemma":[0.9997429,0.00002982195,0.000076416734,0.000039553768,0.00002340388,0.000087936],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019255586,0.0002516415,0.0002812634,0.0004330505,0.00032767988,0.00042625153,0.00029339074,0.00021598031,0.0008631817],"category_scores_gemma":[0.00035836012,0.0003052878,0.00022590409,0.00018463275,0.0002756418,0.00023259324,0.00066245015,0.00021647429,0.0002546801],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039677322,0.00012560344,0.8326113,0.00003975855,0.0001709597,0.00019313113,0.0003677435,0.0039159735,0.15433078,0.00048611258,0.00062072225,0.0067410516],"study_design_scores_gemma":[0.000019985515,0.000059508366,0.99040514,0.0000033294962,0.000024731402,0.000065333035,0.00009339686,0.0068694316,0.0020553956,0.00009815342,0.00029565435,0.000009928993],"about_ca_topic_score_codex":0.006834586,"about_ca_topic_score_gemma":0.008733582,"teacher_disagreement_score":0.006834586,"about_ca_system_score_codex":0.00029324729,"about_ca_system_score_gemma":0.00014581042,"threshold_uncertainty_score":0.013589621},"labels":[],"label_agreement":null},{"id":"W4413488780","doi":"10.3847/1538-4357/adeb51","title":"CHIME All-sky Multiday Pulsar Stacking Search (CHAMPSS): System Overview and First Discoveries","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; McGill Space Institute; Alliance de recherche numérique du Canada; University of Toronto; Canada Foundation for Innovation; Smithsonian Astrophysical Observatory; Canada Excellence Research Chairs, Government of Canada; Commonwealth Scientific and Industrial Research Organisation; McGill University; Canadian Institute for Advanced Research; National Science Foundation","keywords":"Physics; Astronomy; Pulsar; Sky; Astrophysics; Astrobiology","score_opus":0.01730452566045732,"score_gpt":0.33031891608854447,"score_spread":0.31301439042808715,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413488780","genre_codex":"dataset","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.20599055,0.029425804,0.17945184,0.008943879,0.0014768325,0.0066959187,0.22738504,0.20369864,0.1369316],"genre_scores_gemma":[0.28958315,0.005573618,0.3453594,0.0019876913,0.0004906234,0.0019606901,0.321425,0.005596839,0.028023012],"study_design_codex":"not_applicable","study_design_gemma":"observational","domain_scores_codex":[0.9983908,0.000115321134,0.00003191909,0.00031325538,0.0007573226,0.00039145688],"domain_scores_gemma":[0.9978296,0.00008329945,0.00006307339,0.00027235298,0.0011102881,0.0006414108],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0038924613,0.0014301547,0.0009418717,0.0036825305,0.0019455105,0.003333629,0.0024056744,0.0010527134,0.0071038906],"category_scores_gemma":[0.0028575489,0.0011404662,0.00063642865,0.004502426,0.0008793435,0.0021523938,0.003325763,0.0013645068,0.0051905527],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0018664271,0.00026251504,0.06422155,0.0008297558,0.0005004848,0.00036866867,0.0009979486,0.007914267,0.034694076,0.008300521,0.49900723,0.3810366],"study_design_scores_gemma":[0.00043987748,0.00050921825,0.078290254,0.00033582211,0.00024866546,0.0006002587,0.0006217582,0.059827615,0.023964077,0.0038923388,0.83078474,0.00048534418],"about_ca_topic_score_codex":0.40587392,"about_ca_topic_score_gemma":0.45859155,"teacher_disagreement_score":0.40587392,"about_ca_system_score_codex":0.007054867,"about_ca_system_score_gemma":0.010468321,"threshold_uncertainty_score":0.8070229},"labels":[],"label_agreement":null},{"id":"W4413544192","doi":"10.3847/1538-4357/adf1a4","title":"An All-sky Survey of White Dwarf Merger Remnants: Far-Ultraviolet Is the Key","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Nuclear Safety and Security Commission; Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration; Ministério da Ciência, Tecnologia, Inovações e Comunicações; National Science Foundation; Korea Astronomy and Space Science Institute; Smithsonian Institution","keywords":"Physics; White dwarf; Sky; Astronomy; Far ultraviolet; Astrophysics; Stars; Key (lock); Ultraviolet astronomy; Ultraviolet; Astronomical spectroscopy; Spectral line; Optics","score_opus":0.016370765723478564,"score_gpt":0.262743837837628,"score_spread":0.24637307211414944,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413544192","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9972345,0.0002636094,0.00034628093,0.000022352737,0.0000020169655,0.0000065334793,0.0011148355,0.000029986382,0.0009797604],"genre_scores_gemma":[0.9977036,0.000097451164,0.00041219118,0.000017934792,0.0000066472685,0.0000030056688,0.0013534459,0.0000058144237,0.00039998168],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99984086,0.000019741989,0.0000120691075,0.000051280473,0.00004763088,0.000028358281],"domain_scores_gemma":[0.99948823,0.0000373193,0.0001822097,0.00004620442,0.00008132207,0.00016466361],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027061536,0.00013645427,0.00017957111,0.0013360432,0.00030055645,0.00035352723,0.00018433828,0.00012128741,0.0014418439],"category_scores_gemma":[0.00036026535,0.00009535461,0.0001651029,0.00076809013,0.00012992784,0.0003019644,0.0004580369,0.000114641785,0.00048239177],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00002752139,0.000014480448,0.9877885,0.000013735148,0.00002364681,0.000054253465,0.00011611185,0.000048144946,0.0065876646,0.000056972156,0.0002576044,0.00501132],"study_design_scores_gemma":[9.565266e-7,0.000016712638,0.9986482,0.0000032530295,0.000006164282,0.00009087402,0.00011375709,0.00010821784,0.00041990014,0.000020880163,0.00056993956,0.0000011791088],"about_ca_topic_score_codex":0.004630639,"about_ca_topic_score_gemma":0.009483227,"teacher_disagreement_score":0.004630639,"about_ca_system_score_codex":0.00011941202,"about_ca_system_score_gemma":0.00010866694,"threshold_uncertainty_score":0.009207368},"labels":[],"label_agreement":null},{"id":"W4413671341","doi":"10.3847/1538-4357/adf7ac","title":"Spectral Energy Distribution Fitting of Globular Clusters in NGC 4874: Masses and Metallicities","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Physics; Globular cluster; Astrophysics; Spectral energy distribution; Energy distribution; Mass distribution; Astronomy; Galaxy","score_opus":0.005958763216852598,"score_gpt":0.2149976699756383,"score_spread":0.2090389067587857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413671341","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943599,0.00002769727,0.0032437749,0.0000147579785,0.0000023586183,0.0000125910665,0.00072077464,0.0005113207,0.001106735],"genre_scores_gemma":[0.994772,0.000016854628,0.0034887306,0.0000058303062,0.0000020897883,0.000011704671,0.0010940925,0.000067538786,0.00054099225],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998951,0.000013964084,0.000006060214,0.000036165748,0.000026083195,0.000022609727],"domain_scores_gemma":[0.99965,0.00008641156,0.000056980494,0.000054110147,0.00011383591,0.000038665916],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026371132,0.00037586727,0.00021594428,0.001728379,0.0003610713,0.00028570773,0.00037271835,0.00023399635,0.0025495272],"category_scores_gemma":[0.001084513,0.000110205954,0.00029461566,0.001109038,0.0001211933,0.00018552746,0.0002782044,0.00015018342,0.00079198193],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002846108,0.00010588555,0.8361378,0.000051389878,0.00021034494,0.00034516657,0.00038968114,0.08055522,0.033752743,0.00094408705,0.0032387634,0.04398434],"study_design_scores_gemma":[0.00001985205,0.00007455877,0.83403665,0.000008600279,0.00005644778,0.00015599486,0.00026792474,0.14531115,0.016235914,0.00081935956,0.0029851294,0.00002837252],"about_ca_topic_score_codex":0.017169137,"about_ca_topic_score_gemma":0.018716522,"teacher_disagreement_score":0.017169137,"about_ca_system_score_codex":0.0007138399,"about_ca_system_score_gemma":0.00025192095,"threshold_uncertainty_score":0.03413844},"labels":[],"label_agreement":null},{"id":"W4413685489","doi":"10.3847/1538-4357/aded91","title":"Cluster Lensing Mass Inversion (CLUMI+): Combining Dynamics and Weak Lensing around Galaxy Clusters","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"National Science and Technology Council; Academia Sinica","keywords":"Physics; Weak gravitational lensing; Galaxy cluster; Astrophysics; Cluster (spacecraft); Strong gravitational lensing; Brightest cluster galaxy; Gravitational lens; Astronomy; Galaxy; Redshift","score_opus":0.00692374738600819,"score_gpt":0.21169917687332215,"score_spread":0.20477542948731398,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413685489","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.45997104,0.00028050144,0.5296388,0.0004943661,0.000061778,0.00010246919,0.00086021295,0.0042652967,0.004325441],"genre_scores_gemma":[0.8838845,0.000042762975,0.114216775,0.00011570022,0.000035420926,0.00004567275,0.0007399953,0.0003530894,0.0005660907],"study_design_codex":"simulation_or_modeling","study_design_gemma":"observational","domain_scores_codex":[0.99965405,0.00012002288,0.000013760028,0.00007649387,0.00008073139,0.00005498838],"domain_scores_gemma":[0.9988669,0.0003214642,0.000253157,0.00025333668,0.00013772113,0.00016739087],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0016811835,0.0008958345,0.00060144655,0.0009767314,0.00070776645,0.0011879746,0.0022053143,0.0007266866,0.001024241],"category_scores_gemma":[0.004706976,0.0006145285,0.00078124437,0.00061366544,0.0006737107,0.001065835,0.0028282944,0.0008228963,0.00026236387],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00022640165,0.000056678567,0.02926682,0.000071753726,0.00021292697,0.0002417353,0.00016095089,0.9176402,0.011555902,0.010545601,0.0012939749,0.028727042],"study_design_scores_gemma":[0.000015611147,0.000016532967,0.0013337027,0.0000040827476,0.0000072817693,0.000028407261,0.000015010861,0.9942931,0.0015296855,0.0023659044,0.0003766329,0.000014069349],"about_ca_topic_score_codex":0.014067853,"about_ca_topic_score_gemma":0.010652857,"teacher_disagreement_score":0.014067853,"about_ca_system_score_codex":0.00089620036,"about_ca_system_score_gemma":0.0014988319,"threshold_uncertainty_score":0.027971923},"labels":[],"label_agreement":null},{"id":"W4413803241","doi":"10.3847/1538-4357/adf32a","title":"CANUCS/Technicolor: JWST Medium-band Photometry Finds Half of the Star Formation at <i>z</i> &gt; 7.5 Is Obscured","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Javna Agencija za Raziskovalno Dejavnost RS; Canadian Space Agency; National Research Foundation; Space Telescope Science Institute; Canarie; Canadian Foundation for AIDS Research; Danmarks Grundforskningsfond; National Aeronautics and Space Administration","keywords":"Physics; Astrophysics; Galaxy; Redshift; Star formation; Astronomy; Interstellar medium; Photometry (optics); Luminous infrared galaxy; Hubble Ultra-Deep Field; Extinction (optical mineralogy); Hubble Deep Field; Stars","score_opus":0.006145400540539126,"score_gpt":0.21276527416053273,"score_spread":0.2066198736199936,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413803241","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96684587,0.00042927358,0.0008660201,0.00017920745,0.000013242407,0.000018312605,0.014674486,0.00040710226,0.016566623],"genre_scores_gemma":[0.98664004,0.00008257611,0.00044663434,0.000041735228,0.000013398511,0.0000047315098,0.011743106,0.00003547807,0.0009922539],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99941266,0.00005568024,0.000015610749,0.00010950553,0.00016762629,0.00023896134],"domain_scores_gemma":[0.99829,0.00013414255,0.00051295676,0.00031763065,0.00025693214,0.0004883249],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003902343,0.00028855968,0.0002497099,0.0033777135,0.00058830983,0.00108966,0.00059780554,0.0002193638,0.006382847],"category_scores_gemma":[0.0012438714,0.00013067009,0.000227023,0.003859015,0.00044046264,0.000268792,0.00073970685,0.00022912539,0.0013904189],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000625446,0.000029891662,0.9694502,0.000027119844,0.00004540723,0.00007510493,0.0001286237,0.00037119564,0.0019134578,0.0004912294,0.01053219,0.016872989],"study_design_scores_gemma":[0.0000049577247,0.000012307557,0.9944734,0.000009364238,0.000015643594,0.00007437542,0.000080488746,0.00065745274,0.0007115002,0.00005847767,0.0038977629,0.0000042537467],"about_ca_topic_score_codex":0.12852237,"about_ca_topic_score_gemma":0.18787853,"teacher_disagreement_score":0.12852237,"about_ca_system_score_codex":0.0007463209,"about_ca_system_score_gemma":0.000487693,"threshold_uncertainty_score":0.25554854},"labels":[],"label_agreement":null},{"id":"W4413804015","doi":"10.3847/1538-4357/ade4c0","title":"Transient Blurring of the Scintillation Arc of Pulsar B1737+13","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada; National Science Foundation","keywords":"Physics; Pulsar; Scintillation; Line-of-sight; Very-long-baseline interferometry; Lens (geology); Astrophysics; Sky; Curvature; Optics; Position angle; Astronomy; Geometry; Detector","score_opus":0.00848671038711622,"score_gpt":0.30166108856923196,"score_spread":0.2931743781821157,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413804015","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99509287,0.00016188866,0.0029918663,0.00004648621,0.000013115565,0.0000066395173,0.00021754604,0.00019741958,0.0012721774],"genre_scores_gemma":[0.9984617,0.00004322063,0.0010339976,0.000009114764,0.0000058540695,0.0000034789327,0.00023707026,0.0000261081,0.00017945487],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992025,0.000007003208,0.000003446125,0.000022760787,0.000025128027,0.000021404037],"domain_scores_gemma":[0.9997224,0.00005154646,0.00008090425,0.000050656643,0.00004928655,0.000045140194],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017700519,0.00022089492,0.00023936464,0.0007491479,0.000310324,0.0004900953,0.00021440453,0.00022292144,0.0012427322],"category_scores_gemma":[0.00061364763,0.00016017517,0.00026057742,0.0006647079,0.00026471115,0.00021139099,0.00039037716,0.0003738598,0.00021340213],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092309166,0.00012968165,0.46182042,0.00024944518,0.0002287822,0.0023923386,0.0010513508,0.020356901,0.41432497,0.0022116392,0.0029360407,0.09337539],"study_design_scores_gemma":[0.000021259868,0.00015691218,0.92996055,0.000021210111,0.000056982604,0.00066517934,0.00016518618,0.03228532,0.033116136,0.00050898927,0.0030104637,0.00003182181],"about_ca_topic_score_codex":0.0033862994,"about_ca_topic_score_gemma":0.003258902,"teacher_disagreement_score":0.0033862994,"about_ca_system_score_codex":0.0003301565,"about_ca_system_score_gemma":0.00024006859,"threshold_uncertainty_score":0.006733179},"labels":[],"label_agreement":null},{"id":"W4413875564","doi":"10.3847/1538-4357/adf4ea","title":"Development of 1D Non-ideal MHD Simulation Code Towards understanding Long-term Evolution of Protoplanetary Disk","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Western University","funders":"Japan Society for the Promotion of Science","keywords":"Physics; Magnetohydrodynamics; Term (time); Protoplanetary disk; Astrophysics; Code (set theory); Ideal (ethics); Accretion disc; Astronomy; Planet; Plasma; Nuclear physics","score_opus":0.025065030956381015,"score_gpt":0.2819381869829,"score_spread":0.256873156026519,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413875564","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.53786325,0.00066687644,0.4360586,0.0007687261,0.0002502211,0.00045915908,0.0011407469,0.004021507,0.018770965],"genre_scores_gemma":[0.809647,0.0004073974,0.1860468,0.00011720743,0.000041839292,0.00040756975,0.0007473641,0.0003125986,0.0022722161],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9998864,0.000033780434,0.0000068458507,0.000017568518,0.000036760786,0.000018730076],"domain_scores_gemma":[0.9996747,0.00009610301,0.000028349185,0.00003198862,0.00012067349,0.000048169488],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039201375,0.00054639106,0.0004432901,0.00032148804,0.00056110293,0.00057021406,0.0013310214,0.0006227835,0.0015486504],"category_scores_gemma":[0.0009476001,0.0002881146,0.0005760517,0.0002631816,0.0003671019,0.00052312657,0.000758038,0.000671842,0.00025412295],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003602627,0.000057972833,0.0036366668,0.00006175656,0.000030448926,0.000113130096,0.000079281424,0.98148453,0.0045964695,0.0039751614,0.0005768135,0.0053517516],"study_design_scores_gemma":[0.0000111767,0.0000051420598,0.00017269961,0.0000023871644,0.0000022276045,0.0000042068964,0.000004191331,0.9988009,0.00041611417,0.00024167323,0.0003369305,0.000002321663],"about_ca_topic_score_codex":0.009337664,"about_ca_topic_score_gemma":0.0032340367,"teacher_disagreement_score":0.009337664,"about_ca_system_score_codex":0.00049234426,"about_ca_system_score_gemma":0.0010507436,"threshold_uncertainty_score":0.018566608},"labels":[],"label_agreement":null},{"id":"W4413903915","doi":"10.3847/1538-4357/adef01","title":"Massive Interacting Binaries Enhance Feedback in Star-forming Regions","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Astrophysics Division; Office of Advanced Cyberinfrastructure; Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Nuclear Safety and Security Commission; Nederlandse Organisatie voor Wetenschappelijk Onderzoek; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Star (game theory); Astrophysics; Astronomy; Stars","score_opus":0.009653092712345357,"score_gpt":0.2709523211564108,"score_spread":0.26129922844406545,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413903915","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98711604,0.00007674788,0.008969909,0.00011117764,0.000027991495,0.000021499887,0.000056136025,0.00015412041,0.0034664215],"genre_scores_gemma":[0.9982791,0.000025877991,0.0011565934,0.00002443916,0.0000061739443,0.000008601481,0.000016312515,0.000022952247,0.00045998208],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990404,0.000027431797,0.000003231995,0.000013005925,0.000021713504,0.000030544765],"domain_scores_gemma":[0.9995939,0.00015603898,0.000060283186,0.000023763114,0.000044546152,0.00012146129],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032164654,0.00044678533,0.00050384464,0.00029818466,0.000660927,0.00088391884,0.00087232474,0.0005580231,0.0022695994],"category_scores_gemma":[0.0013528257,0.00028710032,0.00041020496,0.00019076896,0.00060550036,0.0007734553,0.0011718264,0.0005813858,0.00014611718],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008888904,0.00009605122,0.0071457396,0.000022842574,0.000049213362,0.00015655403,0.000104289466,0.98097116,0.0062251785,0.0035319282,0.00023055622,0.0013775881],"study_design_scores_gemma":[0.00003849129,0.000050110644,0.0015320992,0.000003654383,0.000011756387,0.000017292394,0.00002473178,0.99662447,0.00076207303,0.0007271169,0.0002022319,0.0000061320275],"about_ca_topic_score_codex":0.014880576,"about_ca_topic_score_gemma":0.008815024,"teacher_disagreement_score":0.014880576,"about_ca_system_score_codex":0.0011019701,"about_ca_system_score_gemma":0.0006748317,"threshold_uncertainty_score":0.029587924},"labels":[],"label_agreement":null},{"id":"W4413956024","doi":"10.3847/1538-4357/adef11","title":"The Atacama Cosmology Telescope: Machine-learning-driven Tools for Detecting Millimeter Sources in Timestream Preprocessing","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Radio Astronomy Observations and Technology","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"Agencia Nacional de Investigación y Desarrollo; National Aeronautics and Space Administration","keywords":"Physics; Cosmology; Astronomy; Millimeter; Telescope; Astrophysics; Preprocessor; Astroparticle physics; Artificial intelligence","score_opus":0.010996023740760408,"score_gpt":0.24938411303328903,"score_spread":0.2383880892925286,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413956024","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.020194124,0.00014277322,0.91057533,0.00019427548,0.00006882696,0.00011112787,0.0024407387,0.06473827,0.0015345543],"genre_scores_gemma":[0.12604038,0.00008629457,0.86234033,0.00017144415,0.00007390012,0.00031871113,0.0070875413,0.0020011966,0.0018801313],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999553,0.000060276925,0.000034547113,0.00012301793,0.00017970927,0.0000493906],"domain_scores_gemma":[0.9984484,0.00045502707,0.00021659728,0.00038955398,0.00037926267,0.000111225294],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00096071156,0.0008336119,0.00054858904,0.0018360418,0.0005588865,0.0011178092,0.0015831189,0.00066163845,0.0040338454],"category_scores_gemma":[0.0038626774,0.00042700168,0.0006383896,0.0013982581,0.0003645988,0.0009153765,0.0010128606,0.0011604296,0.003875297],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005009439,0.00035894776,0.021844897,0.0002482422,0.00024602443,0.00032732566,0.00032746932,0.05531084,0.10571448,0.006333102,0.054559864,0.7542279],"study_design_scores_gemma":[0.00005195323,0.00005942084,0.012922535,0.0000192788,0.000019399124,0.00011212462,0.00007885868,0.91274476,0.043912426,0.009575298,0.020444885,0.000059085185],"about_ca_topic_score_codex":0.005087721,"about_ca_topic_score_gemma":0.008144503,"teacher_disagreement_score":0.005087721,"about_ca_system_score_codex":0.0005932508,"about_ca_system_score_gemma":0.0011536716,"threshold_uncertainty_score":0.013494492},"labels":[],"label_agreement":null},{"id":"W4413977737","doi":"10.3847/1538-4357/adef0d","title":"Massive Extremely High-velocity Outflow in the Quasar J164653.72+243942.2","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Mila - Quebec Artificial Intelligence Institute; Université de Montréal; York University","funders":"","keywords":"Physics; Quasar; Outflow; Astrophysics; Astronomy; Galaxy; Meteorology","score_opus":0.00880246870906851,"score_gpt":0.22193328726562622,"score_spread":0.21313081855655772,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413977737","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984262,0.00012510452,0.0002629544,0.000020655722,0.0000054921024,0.000005949659,0.00043726788,0.000056346278,0.0006601056],"genre_scores_gemma":[0.9985777,0.000030166293,0.0003039673,0.000021655935,0.000012722735,0.0000047025164,0.0008277492,0.000008111849,0.0002132071],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998803,0.000014033379,0.000005571604,0.000025866606,0.00002692378,0.00004726785],"domain_scores_gemma":[0.9996419,0.000027746079,0.0001288894,0.000023218161,0.00003424635,0.00014393989],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000282536,0.00038369888,0.00033876477,0.0014600396,0.00043495774,0.00054186565,0.00023356303,0.0002787202,0.0010136439],"category_scores_gemma":[0.0002331523,0.00015133184,0.00026655284,0.0008153462,0.00020212655,0.00015412291,0.00041506722,0.00023739997,0.00030376358],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003445726,0.00027403323,0.9069017,0.000065434266,0.00023732659,0.0031315358,0.00030818494,0.0013845455,0.07206298,0.00036540622,0.0017697836,0.013154474],"study_design_scores_gemma":[0.000012255695,0.000050821996,0.99727625,0.0000033463182,0.000025898955,0.00030807627,0.00007743054,0.00059981627,0.0008026719,0.000048543316,0.00078761124,0.000007309205],"about_ca_topic_score_codex":0.004292985,"about_ca_topic_score_gemma":0.0048567215,"teacher_disagreement_score":0.004292985,"about_ca_system_score_codex":0.00022818947,"about_ca_system_score_gemma":0.00011285999,"threshold_uncertainty_score":0.008536041},"labels":[],"label_agreement":null},{"id":"W4413998719","doi":"10.3847/1538-4357/adf222","title":"One Year of SN 2023ixf: Breaking through the Degenerate Parameter Space in Light-curve Models with Pulsating Progenitors","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Agencia Estatal de Investigación; Consejo Superior de Investigaciones Científicas; European Commission; Ministerio de Ciencia e Innovación; Generalitat de Catalunya; U.S. Department of Energy; John Templeton Foundation; National Natural Science Foundation of China; York University; Heising-Simons Foundation; Space Telescope Science Institute; Office of Science; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; Johns Hopkins University; Carnegie Mellon University; Harvard University; Ohio State University; Flatiron Health; University of Arizona; Tencent; New Mexico State University; University of Portsmouth; Vanderbilt University; National Science Foundation","keywords":"Physics; Light curve; Parameter space; Degenerate energy levels; Space (punctuation); Astrophysics; Astronomy; Stars; Quantum mechanics; Statistics","score_opus":0.016067146286853292,"score_gpt":0.24001808373935146,"score_spread":0.22395093745249817,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4413998719","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99648845,0.000032684573,0.0022585902,0.00003214825,0.0000037203865,0.00000601098,0.00029268564,0.00009235128,0.0007933446],"genre_scores_gemma":[0.9980038,0.000015415711,0.001102741,0.0000109123575,0.0000028487227,0.000009337092,0.0006690781,0.000028171522,0.00015757847],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989736,0.000020708323,0.0000064175442,0.000022192946,0.000022210033,0.000031174575],"domain_scores_gemma":[0.9996376,0.00013951605,0.000053283744,0.00006449664,0.00003655519,0.0000684701],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000487663,0.0003145567,0.0003525349,0.00038056905,0.00044010027,0.0007657417,0.0006299681,0.0003962557,0.0013212721],"category_scores_gemma":[0.0012262126,0.00019501404,0.00073836173,0.00041171303,0.00032263392,0.00036042507,0.00045614957,0.00030174223,0.00014543829],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004186452,0.00013047973,0.21905823,0.000041923147,0.00016707243,0.0005390249,0.00014028983,0.75849926,0.0050376216,0.0053684306,0.0012319848,0.00936708],"study_design_scores_gemma":[0.000048954502,0.00007820848,0.042912517,0.000009053686,0.00002209336,0.00016435819,0.000075716285,0.95213646,0.0017052558,0.0022316568,0.0005982838,0.000017422835],"about_ca_topic_score_codex":0.013734297,"about_ca_topic_score_gemma":0.009816183,"teacher_disagreement_score":0.013734297,"about_ca_system_score_codex":0.0008644488,"about_ca_system_score_gemma":0.00041162164,"threshold_uncertainty_score":0.027308762},"labels":[],"label_agreement":null},{"id":"W4414026437","doi":"10.3847/1538-4357/adf6ab","title":"Pavo: Stellar Feedback in Action in a Low-mass Dwarf Galaxy","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; Queen's University","funders":"Natural Sciences and Engineering Research Council of Canada; Ministero degli Affari Esteri e della Cooperazione Internazionale; University of Toronto; Bundesministerium für Bildung und Forschung; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Research Foundation; Department of Science and Technology, Ministry of Science and Technology, India; National Aeronautics and Space Administration; National Science Foundation","keywords":"Physics; Dwarf galaxy; Astrophysics; Action (physics); Astronomy; Galaxy","score_opus":0.01099380746332563,"score_gpt":0.2433850738290052,"score_spread":0.23239126636567958,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414026437","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99788135,0.00007651312,0.0003378713,0.00006385197,0.0000037817024,0.000001901677,0.000068398316,0.00009169839,0.0014745597],"genre_scores_gemma":[0.9996711,0.000008332,0.00007766216,0.0000086831915,0.0000016090285,6.1903853e-7,0.000039821996,0.000006051973,0.00018602416],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999144,0.000008597842,0.000002645594,0.000026813335,0.000016825008,0.000030787676],"domain_scores_gemma":[0.9996793,0.000032663178,0.000057062436,0.000029138135,0.000018870584,0.00018300353],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015535759,0.0001773397,0.00024060778,0.00026511148,0.00036007358,0.0006619573,0.0003045166,0.00027585478,0.0014712582],"category_scores_gemma":[0.00067171396,0.00016311764,0.000111883084,0.00012430071,0.0004084056,0.00032097078,0.0008215577,0.0002423992,0.00036138966],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005978759,0.000086558815,0.81623185,0.00009267199,0.000061612336,0.000948336,0.0009576543,0.004875886,0.1456242,0.0046641286,0.0016229912,0.02423623],"study_design_scores_gemma":[0.000034704026,0.00016495184,0.9727595,0.0000151892855,0.000035898476,0.0005132815,0.0004745179,0.013021136,0.006724623,0.0033169081,0.0029144483,0.000024760324],"about_ca_topic_score_codex":0.0028601598,"about_ca_topic_score_gemma":0.003331423,"teacher_disagreement_score":0.0028601598,"about_ca_system_score_codex":0.0004440613,"about_ca_system_score_gemma":0.0001673469,"threshold_uncertainty_score":0.005687058},"labels":[],"label_agreement":null},{"id":"W4414090038","doi":"10.3847/1538-4357/adf723","title":"A Galactic Self-portrait: Density Structure and Integrated Properties of the Milky Way Disk","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute","keywords":"Milky Way; Metallicity; Stellar density; Thick disk; Stars; Disc; Stellar mass; Thin disk; Stellar evolution","score_opus":0.0065667425998105836,"score_gpt":0.1965748526335047,"score_spread":0.1900081100336941,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414090038","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9980325,0.00007284928,0.00056113844,0.000019623803,8.00063e-7,0.0000013620697,0.00035207646,0.0000341081,0.00092548603],"genre_scores_gemma":[0.9989736,0.000026205573,0.00026002765,0.0000028721508,0.0000016247151,0.0000010057212,0.00045854607,0.00000774913,0.00026826546],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999646,0.000006083869,0.000001630725,0.000012856062,0.00000895539,0.000005812813],"domain_scores_gemma":[0.99976414,0.000065560926,0.00004918437,0.000038984253,0.000048290407,0.000033873206],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010286869,0.00006182251,0.00008438686,0.0009176286,0.00009808556,0.0004890434,0.00017450823,0.00011524813,0.001136667],"category_scores_gemma":[0.00070896774,0.000073453295,0.00012865542,0.0005891827,0.00012234737,0.0003405949,0.00022792068,0.00008398723,0.00026542254],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059714417,0.00001660379,0.96607155,0.000014608577,0.00007124647,0.00013678703,0.00059811276,0.0063094315,0.0061035873,0.0007760347,0.0008896069,0.018952616],"study_design_scores_gemma":[0.000001858418,0.000010728371,0.9839686,0.0000037327625,0.000008972178,0.00012145707,0.0002297172,0.013368257,0.0009271187,0.00027955262,0.0010750566,0.0000050610543],"about_ca_topic_score_codex":0.0087171225,"about_ca_topic_score_gemma":0.0089885285,"teacher_disagreement_score":0.0087171225,"about_ca_system_score_codex":0.00024009055,"about_ca_system_score_gemma":0.000049244387,"threshold_uncertainty_score":0.017332733},"labels":[],"label_agreement":null},{"id":"W4414098759","doi":"10.3847/1538-4357/adfee0","title":"Erratum: “Tripling the Census of Dwarf AGN Candidates Using DESI Early Data” (2025, ApJ, 982, 10)","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Insurance, Mortality, Demography, Risk Management","field":"Social Sciences","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Census; Stars; Background radiation; Dwarf galaxy; Field (mathematics)","score_opus":0.0482900178459537,"score_gpt":0.33944456861697214,"score_spread":0.2911545507710184,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414098759","genre_codex":"editorial","genre_gemma":"other","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"other","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.0024535863,0.002483927,0.0015681542,0.09907256,0.7866898,0.0002457169,0.06874246,0.0034029102,0.03534091],"genre_scores_gemma":[0.0225288,0.007190736,0.012526464,0.11685122,0.17826588,0.0007617715,0.18390013,0.0055025397,0.47247252],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.99700516,0.00026719278,0.00042220255,0.00029689685,0.0017524075,0.00025617602],"domain_scores_gemma":[0.9776063,0.0021348638,0.0020290622,0.0012287933,0.015039942,0.001961031],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0025679388,0.0019660299,0.0010254957,0.006735681,0.0035250278,0.0041717775,0.0017168123,0.003356596,0.08483083],"category_scores_gemma":[0.019495463,0.0008031276,0.0014442331,0.0035833335,0.0010261075,0.002653737,0.0022730485,0.0054161036,0.089049906],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000016636972,0.0000047661265,0.00020005008,0.000023163662,0.0000025820202,0.000026660678,0.000004435296,0.000011060396,0.000050536175,0.00010057183,0.99764556,0.0019139799],"study_design_scores_gemma":[0.000034439807,0.000033431916,0.00551406,0.00015263092,0.000021068903,0.00012330925,0.00010229952,0.00013372002,0.00045928004,0.00043159173,0.99294996,0.000044241966],"about_ca_topic_score_codex":0.032190736,"about_ca_topic_score_gemma":0.048535082,"teacher_disagreement_score":0.08483083,"about_ca_system_score_codex":0.003242901,"about_ca_system_score_gemma":0.004640659,"threshold_uncertainty_score":0.28378737},"labels":[],"label_agreement":null},{"id":"W4414136249","doi":"10.3847/1538-4357/adf851","title":"Meridional Circulation Molecular-weighted","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"The Scarborough Hospital; University of Toronto","funders":"University of Toronto; Kavli Institute for Theoretical Physics, University of California, Santa Barbara; National Science Foundation","keywords":"Angular momentum; Differential rotation; Rossby number; Meridional flow; Turbulence; Zonal and meridional; Magnetohydrodynamics; Nonlinear system; Rossby wave","score_opus":0.006730904187740949,"score_gpt":0.22624726013274585,"score_spread":0.2195163559450049,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414136249","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98461074,0.00005742481,0.008082442,0.00016447708,0.000014843551,0.0000063612806,0.00016444037,0.000092843795,0.0068064756],"genre_scores_gemma":[0.9980691,0.000024802519,0.00059511885,0.000017863527,0.000004232803,0.000001974481,0.0000593435,0.0000137066345,0.0012138363],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99998057,0.0000025440813,9.568514e-7,0.000005928274,0.0000035058565,0.000006550908],"domain_scores_gemma":[0.9999324,0.0000067022465,0.000021089485,0.000007687293,0.000016220743,0.000015943626],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000039527873,0.00015354877,0.00010957021,0.00015511794,0.00021244815,0.0006423377,0.00024349133,0.00016228193,0.0022437025],"category_scores_gemma":[0.00033826922,0.00009424506,0.00012870891,0.00010736103,0.00026367363,0.00043094862,0.00031243736,0.00023487769,0.00021528742],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036267054,0.00014959318,0.07329557,0.00011439514,0.00013027222,0.00055764604,0.00040238336,0.64308876,0.17900464,0.06883026,0.002480981,0.031582844],"study_design_scores_gemma":[0.000026176853,0.000050241135,0.02331711,0.0000069281236,0.00001470527,0.0000581206,0.000082167535,0.96517974,0.004893399,0.004898336,0.0014511035,0.000021939433],"about_ca_topic_score_codex":0.006406707,"about_ca_topic_score_gemma":0.003776511,"teacher_disagreement_score":0.006406707,"about_ca_system_score_codex":0.00047629248,"about_ca_system_score_gemma":0.00032234183,"threshold_uncertainty_score":0.012738824},"labels":[],"label_agreement":null},{"id":"W4414136454","doi":"10.3847/1538-4357/adf8dc","title":"PEARLS: Globular Clusters and Ultracompact Dwarfs in the El Gordo Galaxies at <i>z</i> = 0.87","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada; Goddard Space Flight Center; Nuclear Safety and Security Commission; Space Telescope Science Institute; Canadian Institute for Theoretical Astrophysics; National Aeronautics and Space Administration","keywords":"Globular cluster; Galaxy; Redshift; Cluster (spacecraft); Population; Dwarf galaxy; Sequence (biology)","score_opus":0.005507420145355068,"score_gpt":0.22316072944590037,"score_spread":0.2176533093005453,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414136454","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9993555,0.00003195414,0.000027788383,0.000027803386,5.3077633e-7,9.76884e-7,0.000043614695,0.0000040429063,0.0005078367],"genre_scores_gemma":[0.99954456,0.000023950979,0.000053128904,0.00001164831,0.000001099418,6.7859645e-7,0.00008986488,0.0000019002945,0.00027317333],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99996483,0.0000022933664,0.000001152047,0.000011076091,0.000008161726,0.0000124841235],"domain_scores_gemma":[0.9998772,0.0000113753185,0.000041702264,0.000010388547,0.00001390165,0.000045392146],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010061896,0.00008159609,0.00013207561,0.0006928177,0.00034764365,0.000477448,0.00017108652,0.00013519566,0.0011224251],"category_scores_gemma":[0.00017783702,0.00008704261,0.000056832636,0.00033945404,0.00049943745,0.00024013796,0.0004509868,0.00012707042,0.00014841699],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000095261654,0.000025911117,0.97917545,0.000013167957,0.000020608655,0.00030928565,0.001174477,0.000114452625,0.010982618,0.0006272153,0.00038730993,0.0070742],"study_design_scores_gemma":[0.000001987192,0.0000069160415,0.99882215,0.000001789105,0.000003315702,0.00007406308,0.0003948984,0.000082951316,0.00018087294,0.00006817379,0.00036161396,0.0000011354016],"about_ca_topic_score_codex":0.025495838,"about_ca_topic_score_gemma":0.04335072,"teacher_disagreement_score":0.025495838,"about_ca_system_score_codex":0.00037959783,"about_ca_system_score_gemma":0.00013811112,"threshold_uncertainty_score":0.050694823},"labels":[],"label_agreement":null},{"id":"W4414137117","doi":"10.3847/1538-4357/adf8e8","title":"Reprocessing of the Parkes 70 cm Survey and Discovery of a New Radio Pulsar in the Large Magellanic Cloud","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Reed College; Commonwealth Scientific and Industrial Research Organisation; Australian Government; Oregon State University; University of Wisconsin-Milwaukee; Kenyon College; Vanderbilt University; Franklin and Marshall College; National Science Foundation","keywords":"Pulsar; Binary pulsar; Pulsar planet; Large Magellanic Cloud; X-ray pulsar; Millisecond pulsar","score_opus":0.01391521013712614,"score_gpt":0.3188743926746017,"score_spread":0.30495918253747556,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414137117","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99742305,0.00012829105,0.0010680848,0.00004145678,0.000014963205,0.000021864384,0.00055594335,0.00023611734,0.0005101905],"genre_scores_gemma":[0.9898977,0.0001330453,0.006784068,0.000094030474,0.00004154994,0.000025765235,0.0024234827,0.00007327083,0.0005270413],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9993105,0.00009445332,0.00004975342,0.00015859507,0.00027704905,0.00010952587],"domain_scores_gemma":[0.9972812,0.00032636465,0.0008479427,0.0006224352,0.00058254186,0.00033961644],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011010545,0.00030745743,0.00037847282,0.0024481427,0.0004100724,0.00064316834,0.00042035,0.000253495,0.000662299],"category_scores_gemma":[0.002034121,0.00027482046,0.0003722152,0.0018387808,0.00027953455,0.0003798152,0.0007357506,0.00036902755,0.00032858676],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00031319633,0.00009446582,0.8777483,0.000082473794,0.00014146393,0.0011163178,0.00065955915,0.00092413794,0.05599428,0.0001474142,0.0015411727,0.061237294],"study_design_scores_gemma":[0.000015243283,0.00008953688,0.98660755,0.000012672778,0.000037650716,0.00044408173,0.00010309997,0.0013882399,0.0072430363,0.000042951993,0.0040043355,0.00001159084],"about_ca_topic_score_codex":0.0057062157,"about_ca_topic_score_gemma":0.012324967,"teacher_disagreement_score":0.0057062157,"about_ca_system_score_codex":0.00039240337,"about_ca_system_score_gemma":0.00038718054,"threshold_uncertainty_score":0.011346042},"labels":[],"label_agreement":null},{"id":"W4414141615","doi":"10.3847/1538-4357/adf2a1","title":"The ATLAS Virtual Research Assistant","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Particle physics theoretical and experimental studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Science and Technology Facilities Council; Queen's University; Nuclear Safety and Security Commission; Space Telescope Science Institute; National Research Foundation; Queen's University Belfast; National Aeronautics and Space Administration","keywords":"Atlas (anatomy); Workload; Sky; Metric (unit); Training set; Decision tree; Facility management","score_opus":0.020759545847552057,"score_gpt":0.33305488831074753,"score_spread":0.31229534246319546,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414141615","genre_codex":"software","genre_gemma":"software","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"software","genre_consensus":"software","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.036633786,0.0014931306,0.29540986,0.004357247,0.0019193783,0.0010614805,0.032464154,0.49471363,0.13194737],"genre_scores_gemma":[0.42775992,0.0010901354,0.33049124,0.0034252,0.0015561549,0.0017125871,0.07125026,0.024949357,0.13776512],"study_design_codex":"not_applicable","study_design_gemma":"not_applicable","domain_scores_codex":[0.9972269,0.00084483094,0.00012645812,0.0007135682,0.0007239259,0.00036427015],"domain_scores_gemma":[0.9930648,0.0015900888,0.00028057102,0.0022473119,0.0012478733,0.001569386],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.003792358,0.0014859197,0.0009166551,0.0016478162,0.0011112193,0.00413155,0.003669844,0.0012512936,0.10079121],"category_scores_gemma":[0.009843938,0.00090145407,0.0009792976,0.001318835,0.00062986906,0.0030542123,0.0056415047,0.0016741474,0.06948228],"study_design_candidate":"not_applicable","study_design_consensus":"not_applicable","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002870674,0.0002784475,0.0071374387,0.00038403974,0.00013178373,0.00066842115,0.0008373608,0.011399347,0.0074782954,0.012636945,0.6301821,0.32599524],"study_design_scores_gemma":[0.00037418326,0.00040241575,0.0025768746,0.00006264242,0.000054375756,0.0004908921,0.00039400958,0.061173555,0.009747615,0.012050004,0.9125432,0.00013028836],"about_ca_topic_score_codex":0.004263173,"about_ca_topic_score_gemma":0.0042721797,"teacher_disagreement_score":0.10079121,"about_ca_system_score_codex":0.0014784638,"about_ca_system_score_gemma":0.0023271788,"threshold_uncertainty_score":0.3371802},"labels":[],"label_agreement":null},{"id":"W4414146158","doi":"10.3847/1538-4357/adf638","title":"Unveiling the Cosmic Gems Arc at <i>z</i> ∼ 10 with JWST NIRCam","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":5,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute","keywords":"Galaxy; Metallicity; Redshift; Star formation; Spectral energy distribution; COSMIC cancer database; Star cluster; Gravitational lens; Stellar mass","score_opus":0.00493396115069151,"score_gpt":0.1995731733192704,"score_spread":0.1946392121685789,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414146158","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9651644,0.00060566544,0.0041330536,0.00044465944,0.00010711408,0.000035715,0.005466459,0.0014901933,0.022552745],"genre_scores_gemma":[0.980903,0.00017729904,0.008900769,0.00022530524,0.0001602252,0.000019191331,0.0074522276,0.00034451848,0.0018174892],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99977297,0.000012199405,0.0000067976366,0.000059622347,0.00009681899,0.00005168291],"domain_scores_gemma":[0.9993973,0.00003357485,0.0001347943,0.00011006187,0.00013219521,0.00019212493],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039526154,0.00026299976,0.00026260284,0.0014132244,0.00036124428,0.00082924345,0.00035824312,0.00024501927,0.0025007627],"category_scores_gemma":[0.0005775149,0.0002925709,0.00042878804,0.00095094694,0.00026290023,0.00042181087,0.0008217307,0.0005314714,0.0009136804],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00093322695,0.00030687285,0.6330301,0.00036886567,0.00053721457,0.0017015996,0.0013053425,0.0057111117,0.19361253,0.0046867128,0.035708994,0.12209744],"study_design_scores_gemma":[0.000032542346,0.00006322695,0.95094496,0.000034667788,0.000105284984,0.00025676537,0.0001436296,0.007398345,0.010274269,0.0006959527,0.03002567,0.00002455203],"about_ca_topic_score_codex":0.00944896,"about_ca_topic_score_gemma":0.024299357,"teacher_disagreement_score":0.00944896,"about_ca_system_score_codex":0.0007134067,"about_ca_system_score_gemma":0.00030364053,"threshold_uncertainty_score":0.01878792},"labels":[],"label_agreement":null},{"id":"W4414146167","doi":"10.3847/1538-4357/adf6b6","title":"Multiwavelength Study of HESS J0632+057: New Insights into Pulsar–Disk Interaction","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"Jet Propulsion Laboratory; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Ministry of Science and ICT, South Korea; Office of Science; Chungbuk National University; National Research Foundation; National Energy Research Scientific Computing Center; U.S. Department of Energy; California Institute of Technology; National Aeronautics and Space Administration; National Research Foundation of Korea; National Science Foundation","keywords":"Pulsar; Flux (metallurgy); Context (archaeology); Phase (matter); Absorption (acoustics); Binary number; Shock (circulatory)","score_opus":0.014287681590331096,"score_gpt":0.27607754690033987,"score_spread":0.26178986531000875,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414146167","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99879587,0.000118937955,0.00011765682,0.000024761235,0.0000042523143,0.0000026125442,0.00015760955,0.000007601709,0.0007706114],"genre_scores_gemma":[0.9988783,0.000043561453,0.00032985889,0.000016667538,0.000012702677,0.0000030641022,0.00052374543,0.0000043222885,0.00018765545],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99990666,0.000008561559,0.0000066579705,0.000023514795,0.000030320414,0.000024248444],"domain_scores_gemma":[0.9997795,0.00003085603,0.00006743048,0.000024377725,0.000031643358,0.000066120585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018486493,0.00015524002,0.00026667843,0.0016402346,0.00033101533,0.0005143831,0.00023566866,0.00032091266,0.000836842],"category_scores_gemma":[0.00028812807,0.00013525588,0.00019607438,0.0010479694,0.00016394064,0.0002982964,0.0005556298,0.00023668603,0.00030559735],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030552517,0.00017753152,0.87911993,0.00007278441,0.000090094305,0.0018473242,0.00059772277,0.000628613,0.098687604,0.00035191595,0.00073928945,0.0173817],"study_design_scores_gemma":[0.0000034368582,0.000029039687,0.99730563,0.0000030889644,0.00000865811,0.0002716972,0.00010989071,0.00053179706,0.0009773654,0.000053926135,0.00070061977,0.0000048720126],"about_ca_topic_score_codex":0.0021724198,"about_ca_topic_score_gemma":0.0057140095,"teacher_disagreement_score":0.0021724198,"about_ca_system_score_codex":0.0002944699,"about_ca_system_score_gemma":0.00015396031,"threshold_uncertainty_score":0.0043195486},"labels":[],"label_agreement":null},{"id":"W4414146169","doi":"10.3847/1538-4357/adf84f","title":"Parallel Collisionless Shocks in Strongly Magnetized Electron–Ion Plasma. I. Temperature Anisotropies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute; University of Waterloo","funders":"Ministero dello Sviluppo Economico; University of Waterloo; Nuclear Safety and Security Commission; Ministerio de Economía y Competitividad; Government of Canada; Institut Périmètre de physique théorique; Innovation, Science and Economic Development Canada; National Aeronautics and Space Administration","keywords":"Magnetohydrodynamic drive; Magnetohydrodynamics; Magnetic field; Anisotropy; Kinetic energy; Ion; Electron; Population; Magnetization; Plasma","score_opus":0.0044439860708254545,"score_gpt":0.22363759980375447,"score_spread":0.219193613732929,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414146169","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9943586,0.00009779896,0.00294745,0.000079171536,0.000014515945,0.000014582769,0.00007096011,0.00007327871,0.0023437547],"genre_scores_gemma":[0.99946755,0.00002668821,0.0003128533,0.000009241918,0.0000033490332,0.000003230393,0.000026344927,0.000007342457,0.0001434794],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999386,0.000010473954,0.0000031091433,0.000010713393,0.000014494998,0.000022552224],"domain_scores_gemma":[0.9998266,0.00003627892,0.00006662008,0.00001532269,0.00001952329,0.00003569039],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00013591666,0.00029058388,0.00024171258,0.00027559607,0.0002480446,0.0006902523,0.00039534183,0.0002582567,0.0008629021],"category_scores_gemma":[0.0007636502,0.00015916348,0.00020342659,0.00019042185,0.00069161935,0.0003665113,0.000678132,0.0003556727,0.000069287744],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012184388,0.00025751186,0.032238048,0.00018788826,0.00016089306,0.0017073796,0.0004329546,0.74646837,0.17852308,0.031011691,0.0010245778,0.0067690825],"study_design_scores_gemma":[0.00012914836,0.00013881244,0.012274888,0.0000120267005,0.000019840234,0.00010563243,0.00010358646,0.9677548,0.01381849,0.005161176,0.00046128104,0.000020217989],"about_ca_topic_score_codex":0.0023676644,"about_ca_topic_score_gemma":0.0007144732,"teacher_disagreement_score":0.0023676644,"about_ca_system_score_codex":0.00034882536,"about_ca_system_score_gemma":0.00025152328,"threshold_uncertainty_score":0.0047078133},"labels":[],"label_agreement":null},{"id":"W4414148087","doi":"10.3847/1538-4357/adf645","title":"Tracing Red Giant Members of the Globular Cluster Palomar 5 with APOGEE and Gaia","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; Ministério da Ciência, Tecnologia e Inovação; University of Oxford; York University; Villum Fonden; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; European Space Agency; Johns Hopkins University; Carnegie Institution of Washington; University of Utah; Ohio State University; Simons Foundation; National Science Foundation; Smithsonian Institution; U.S. Department of Energy; Agencia Nacional de Investigación y Desarrollo; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Globular cluster; Milky Way; Red clump; Red-giant branch; Red giant; Star cluster; Open cluster; Dark matter","score_opus":0.005195103610130352,"score_gpt":0.20476441686845093,"score_spread":0.19956931325832059,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414148087","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992041,0.000023959723,0.00014911384,0.000015630045,0.0000010515168,0.000004081421,0.00008692907,0.000013264184,0.00050183845],"genre_scores_gemma":[0.9991472,0.000010195469,0.00036716167,0.000008479839,0.0000019328297,0.0000028423035,0.00029104314,0.000003287591,0.0001679283],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99980074,0.000023615723,0.000006206384,0.00007155419,0.000055125838,0.000042785272],"domain_scores_gemma":[0.9992772,0.00012437768,0.00022203485,0.00006720893,0.00012709889,0.00018213785],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029607708,0.00017432695,0.00015418185,0.0015591771,0.00038740723,0.00044599196,0.0003365422,0.00027453605,0.00085365353],"category_scores_gemma":[0.0009107058,0.00012844519,0.00014577707,0.00085769146,0.00030266104,0.00028048817,0.00081232167,0.00013930851,0.00031308917],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006158976,0.000017400427,0.99091023,0.000007210072,0.000017346776,0.00017062691,0.00045059022,0.0003376262,0.0032274344,0.00014541714,0.00033618964,0.004318418],"study_design_scores_gemma":[0.0000035196044,0.000027068316,0.99595934,0.000004912068,0.0000079852025,0.00009548378,0.00042596928,0.0022442883,0.00047699155,0.0000731546,0.0006778725,0.0000035447708],"about_ca_topic_score_codex":0.013440351,"about_ca_topic_score_gemma":0.021058338,"teacher_disagreement_score":0.013440351,"about_ca_system_score_codex":0.0004549686,"about_ca_system_score_gemma":0.00016042401,"threshold_uncertainty_score":0.02672422},"labels":[],"label_agreement":null},{"id":"W4414148779","doi":"10.3847/1538-4357/adef38","title":"The Resolved Structure of a Low-metallicity Photodissociation Region","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"National Science and Technology Council; National Astronomical Observatory of Japan; Belgian Federal Science Policy Office; Space Telescope Science Institute; Deutsche Forschungsgemeinschaft; National Institutes of Natural Sciences; National Aeronautics and Space Administration; National Radio Astronomy Observatory; Korea Astronomy and Space Science Institute; National Science Foundation","keywords":"Photodissociation; Metallicity; Milky Way; H II region; Stars; Spectroscopy; Interstellar cloud; Dissociation (chemistry)","score_opus":0.005892071451787333,"score_gpt":0.23299245575513552,"score_spread":0.2271003843033482,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414148779","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99759835,0.00010481444,0.00070798985,0.000030628813,0.0000010000451,0.000004552293,0.0001964274,0.000026978043,0.0013293553],"genre_scores_gemma":[0.99925154,0.000014158659,0.00036802024,0.000009032973,0.0000015632462,0.0000013220089,0.0002035318,0.000004234513,0.00014667174],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99992895,0.000003803909,0.0000026190303,0.000033332402,0.0000096880785,0.000021653372],"domain_scores_gemma":[0.9997476,0.00003728053,0.00009464479,0.000020639178,0.000046856232,0.000053003092],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0000879389,0.00012252752,0.00015535744,0.0004665011,0.00037184087,0.0007684654,0.00027839065,0.00021366579,0.0010883918],"category_scores_gemma":[0.0003154706,0.00016446263,0.0001252436,0.0004193136,0.00027109904,0.00024384889,0.00044756834,0.0001789928,0.00024047657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00026713058,0.00008184988,0.79142874,0.00004496725,0.000059448044,0.0004099928,0.000580327,0.0043835514,0.18061595,0.0016230862,0.00057775446,0.019927213],"study_design_scores_gemma":[0.000013588149,0.000022818565,0.9839612,0.000007228542,0.000017905186,0.00014733637,0.00013919135,0.007516552,0.0067764297,0.0003037373,0.0010864713,0.000007354723],"about_ca_topic_score_codex":0.011902969,"about_ca_topic_score_gemma":0.008187317,"teacher_disagreement_score":0.011902969,"about_ca_system_score_codex":0.0005789351,"about_ca_system_score_gemma":0.00021828162,"threshold_uncertainty_score":0.023667336},"labels":[],"label_agreement":null},{"id":"W4414254051","doi":"10.3847/1538-4357/adf745","title":"Three-component Phase Separation for Ultramassive White Dwarf Models","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University","funders":"","keywords":"Buoyancy; White dwarf; Mixing (physics); Convection; Separation (statistics); Flux (metallurgy); Phase (matter); Current (fluid)","score_opus":0.017889485005144194,"score_gpt":0.28323630785918874,"score_spread":0.26534682285404454,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414254051","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96715957,0.00031668262,0.024896339,0.00047011793,0.00004926725,0.00004365357,0.00057354977,0.0003024641,0.006188415],"genre_scores_gemma":[0.992486,0.000081864346,0.0051014177,0.00007493584,0.00001802361,0.00004903359,0.00035383363,0.00009753549,0.0017374513],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99989307,0.000029741925,0.0000049504397,0.000017792467,0.00002014717,0.00003421551],"domain_scores_gemma":[0.9994642,0.00020865591,0.00010340758,0.00003276952,0.00008284109,0.000108147215],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033704517,0.0006402474,0.0007000117,0.00058479985,0.00071373105,0.00096451864,0.0011086024,0.0014233956,0.0020912755],"category_scores_gemma":[0.0013904301,0.00038751692,0.001024082,0.00033907272,0.00089470093,0.0006589684,0.00096502877,0.0007633399,0.0002173139],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00008084986,0.000060302365,0.00456759,0.000025132062,0.000032059193,0.00010951365,0.00003718595,0.98771244,0.001322244,0.004873841,0.00032190554,0.00085688685],"study_design_scores_gemma":[0.00001905087,0.000007941834,0.00031484445,0.0000028180439,0.000003296211,0.0000056382833,0.000009594922,0.99849343,0.00017447826,0.000808891,0.00015674863,0.0000031972234],"about_ca_topic_score_codex":0.030129774,"about_ca_topic_score_gemma":0.013608157,"teacher_disagreement_score":0.030129774,"about_ca_system_score_codex":0.0013175074,"about_ca_system_score_gemma":0.0010258856,"threshold_uncertainty_score":0.059908748},"labels":[],"label_agreement":null},{"id":"W4414254829","doi":"10.3847/1538-4357/adf743","title":"Precise Parameters for Two LISA Sources","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Particle physics theoretical and experimental studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; NASA Exoplanet Science Institute; National Aeronautics and Space Administration; Nuclear Safety and Security Commission; Space Telescope Science Institute; Smithsonian Institution; National Science Foundation","keywords":"Spectrograph; Interferometry; Amplitude; Hubble space telescope; Space Telescope Imaging Spectrograph; SIGNAL (programming language); Primary (astronomy); Astronomical interferometer; Parameter space","score_opus":0.01141829142628814,"score_gpt":0.28308429663997625,"score_spread":0.2716660052136881,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414254829","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9361454,0.0015397003,0.018575776,0.0007183916,0.00015305275,0.000065191314,0.018875277,0.002223103,0.021704173],"genre_scores_gemma":[0.9710487,0.00014911898,0.008686727,0.00014292408,0.000097500895,0.00004732693,0.018156461,0.0003306819,0.0013406394],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99957055,0.00004517894,0.000034584078,0.00014023796,0.00014559524,0.00006382125],"domain_scores_gemma":[0.99821365,0.00025225326,0.0004713619,0.00047249923,0.00033740603,0.00025294273],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007670789,0.0005305439,0.0006349373,0.0034054741,0.00089715386,0.0015940731,0.00058703753,0.0007302243,0.0035849544],"category_scores_gemma":[0.0024560648,0.00041882944,0.00045014863,0.0027311943,0.00034245403,0.0006848119,0.0013712446,0.000837287,0.0018461926],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0010296154,0.00016424808,0.7801848,0.00023592205,0.00039028583,0.00094881805,0.0010953945,0.024684597,0.047604986,0.018257426,0.02082702,0.10457692],"study_design_scores_gemma":[0.00012269642,0.000057064517,0.88637775,0.00007674625,0.00012028666,0.000663543,0.00028740964,0.042978115,0.0131343445,0.007906318,0.048109904,0.00016588575],"about_ca_topic_score_codex":0.0033932098,"about_ca_topic_score_gemma":0.0045680474,"teacher_disagreement_score":0.0035849544,"about_ca_system_score_codex":0.0012413303,"about_ca_system_score_gemma":0.00043383718,"threshold_uncertainty_score":0.011992872},"labels":[],"label_agreement":null},{"id":"W4414299332","doi":"10.3847/1538-4357/adf6d9","title":"A Magnetic Field Detection in the Massive O-type Bright Giant 63 Oph","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Royal Military College of Canada; Queen's University","funders":"","keywords":"Magnetic field; Balmer series; Stars; Magnetosphere; Dipole; Population; Magnetic dipole; Spectral line","score_opus":0.006193404295358769,"score_gpt":0.22019749359141597,"score_spread":0.2140040892960572,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414299332","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9988451,0.000038184706,0.00012781355,0.000016598968,0.0000026620141,0.0000023118055,0.0001809047,0.000010682293,0.00077570614],"genre_scores_gemma":[0.999241,0.000027199105,0.0001645276,0.000019116183,0.0000057068505,0.0000018437361,0.00035283706,0.0000045366482,0.0001833171],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998944,0.000007743339,0.000008275523,0.000030718053,0.000027726104,0.000031153737],"domain_scores_gemma":[0.9993205,0.000097336735,0.00020992357,0.00005513563,0.000100402016,0.00021666288],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022982268,0.00020925645,0.00018687519,0.0009902503,0.00032025095,0.00039706432,0.00016066052,0.00028623285,0.00096025266],"category_scores_gemma":[0.000679339,0.000086881904,0.000101686535,0.00044518424,0.00033233548,0.00016390733,0.0005001039,0.00015562092,0.00039308664],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00025511885,0.000039170856,0.9090439,0.000033766806,0.00002540887,0.00066509534,0.0002546123,0.000073475065,0.080829,0.00011438022,0.00035457528,0.008311465],"study_design_scores_gemma":[0.000007693147,0.00008058303,0.99213225,0.0000045966544,0.000016082871,0.000717149,0.00012863973,0.00020046798,0.0058304695,0.00008309274,0.000793179,0.0000059314225],"about_ca_topic_score_codex":0.0017848951,"about_ca_topic_score_gemma":0.0023457054,"teacher_disagreement_score":0.0017848951,"about_ca_system_score_codex":0.00015258651,"about_ca_system_score_gemma":0.00009220511,"threshold_uncertainty_score":0.0035490394},"labels":[],"label_agreement":null},{"id":"W4414340346","doi":"10.3847/1538-4357/adf846","title":"The DECam MAGIC Survey: Spectroscopic Follow-up of the Most Metal-poor Stars in the Distant Milky Way Halo<sup>*</sup>","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":10,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Lawrence Berkeley National Laboratory; Fermilab; Laboratory Directed Research and Development; Institut de Física d'Altes Energies; Integrated Electronics Engineering Center, Binghamton University; University of Illinois at Urbana-Champaign; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; National Aeronautics and Space Administration; Coordenação de Aperfeiçoamento de Pessoal de Nível Superior; Ministério da Ciência, Tecnologia e Inovação; Deutsche Forschungsgemeinschaft; Kavli Institute for Cosmological Physics, University of Chicago; Ohio State University; Science and Technology Facilities Council; University College London; Fundação de Amparo à Pesquisa do Estado de São Paulo; Argonne National Laboratory; U.S. Department of Energy; Conselho Nacional de Desenvolvimento Científico e Tecnológico; University of Chicago; National Science Foundation","keywords":"Milky Way; Metallicity; Stars; Galactic halo; Large Magellanic Cloud; Dwarf galaxy; Galaxy; Population; Supernova","score_opus":0.010699233885107346,"score_gpt":0.23546549298993585,"score_spread":0.2247662591048285,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414340346","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9985506,0.00005727235,0.00003994344,0.000015232689,0.0000015168549,0.000004066793,0.00087854295,0.000008188959,0.00044462562],"genre_scores_gemma":[0.9968923,0.00004344935,0.0002734256,0.000026933481,0.0000065185495,0.000008223599,0.0023843911,0.000005342422,0.00035948918],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999001,0.000010512086,0.000008247192,0.000031457905,0.000024076498,0.000025657962],"domain_scores_gemma":[0.99956304,0.000023100998,0.00015172843,0.00004449922,0.00007184217,0.0001458308],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017394955,0.00015391716,0.00017516839,0.0010265958,0.00023573718,0.00029164046,0.0002134064,0.00014997034,0.0010351785],"category_scores_gemma":[0.0003008067,0.00009788093,0.00010677907,0.00053942256,0.000114296854,0.00020554378,0.0005537996,0.00011775054,0.0004147239],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000055310076,0.000011898431,0.99317765,0.0000059501713,0.000010941003,0.000089948255,0.00008779844,0.000013849916,0.0027840966,0.000012266999,0.00028355257,0.003466624],"study_design_scores_gemma":[0.0000016287812,0.0000197961,0.9991079,0.000001109957,0.0000044209287,0.00013734431,0.00006164541,0.000029268153,0.00017716456,0.0000031478744,0.00045560868,9.693209e-7],"about_ca_topic_score_codex":0.0046086665,"about_ca_topic_score_gemma":0.012859855,"teacher_disagreement_score":0.0046086665,"about_ca_system_score_codex":0.00015603562,"about_ca_system_score_gemma":0.00010246699,"threshold_uncertainty_score":0.009163678},"labels":[],"label_agreement":null},{"id":"W4414340350","doi":"10.3847/1538-4357/adf6b7","title":"Validation and Calibration of Semianalytical Models for the Event Horizon Telescope Observations of Sagittarius A*","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto; Perimeter Institute; University of Waterloo","funders":"","keywords":"Event horizon; Accretion (finance); Event (particle physics); Telescope; Calibration; Supermassive black hole; Scattering; Accretion disc","score_opus":0.018493077247678003,"score_gpt":0.25094554447773426,"score_spread":0.23245246723005625,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414340350","genre_codex":"empirical","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9249569,0.00019571271,0.07074025,0.00037969218,0.000036412213,0.000059050064,0.0006985759,0.001117624,0.0018158604],"genre_scores_gemma":[0.99205834,0.000023090637,0.007129912,0.000037999183,0.0000070085925,0.00002135836,0.0005041228,0.00007309943,0.00014510092],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999388,0.00029073318,0.00003188045,0.00016438962,0.000076664306,0.00004822172],"domain_scores_gemma":[0.99449617,0.0036955911,0.0005099577,0.00070283853,0.00040723383,0.00018820095],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0036783393,0.00062607124,0.00041889626,0.0008702547,0.00057626126,0.0012193036,0.001862228,0.0011429219,0.0008535649],"category_scores_gemma":[0.010713419,0.000596024,0.0008171927,0.0005063299,0.0013053935,0.00093065074,0.0009763169,0.0011495666,0.0002873279],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004495366,0.000038309907,0.007997388,0.000016724887,0.000033112246,0.000025182278,0.00004074158,0.98539704,0.00081417564,0.0013022847,0.00025181522,0.0040382375],"study_design_scores_gemma":[0.000007924727,0.000009223475,0.0018904256,0.000004479453,0.0000026119076,0.000009797936,0.0000067490873,0.99682355,0.0004192213,0.0007225174,0.00009782238,0.000005786834],"about_ca_topic_score_codex":0.012824498,"about_ca_topic_score_gemma":0.008255154,"teacher_disagreement_score":0.012824498,"about_ca_system_score_codex":0.002218694,"about_ca_system_score_gemma":0.0008029156,"threshold_uncertainty_score":0.025499701},"labels":[],"label_agreement":null},{"id":"W4414487614","doi":"10.3847/1538-4357/ae0039","title":"The DECam MAGIC Survey: A Wide-field Photometric Metallicity Study of the Sculptor Dwarf Spheroidal Galaxy","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"SLAC National Accelerator Laboratory; Argonne National Laboratory; Integrated Electronics Engineering Center, Binghamton University; Office of Science; European Space Agency; Uppsala Universitet; Institut de Física d'Altes Energies; Universität Wien; Ministério da Ciência, Tecnologia e Inovação; Fundação de Amparo à Pesquisa do Estado de São Paulo; High Energy Physics; Deutsche Forschungsgemeinschaft; Yale University; University of Portsmouth; University of Chicago; Kavli Institute for Cosmological Physics, University of Chicago; Ohio State University; University of Illinois at Urbana-Champaign; Lawrence Berkeley National Laboratory; University of Pennsylvania; Financiadora de Estudos e Projetos; Fundação Carlos Chagas Filho de Amparo à Pesquisa do Estado do Rio de Janeiro; University of Sussex; University College London; National Aeronautics and Space Administration; Fermilab; Laboratory Directed Research and Development; National Science Foundation; Science and Technology Facilities Council; U.S. Department of Energy","keywords":"Metallicity; Milky Way; Galaxy; Dwarf spheroidal galaxy; Stars; Dwarf galaxy","score_opus":0.013354859151440331,"score_gpt":0.25177304205336976,"score_spread":0.23841818290192943,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414487614","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981622,0.00006275255,0.00010566064,0.000011534306,6.546824e-7,0.0000032300468,0.0010397243,0.000019297308,0.0005948852],"genre_scores_gemma":[0.9960383,0.00005376954,0.00047753006,0.000012523757,0.0000055563924,0.0000038631824,0.0031023154,0.000012523015,0.00029369257],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985886,0.000014028287,0.0000068689956,0.000050846233,0.00003784417,0.000031381518],"domain_scores_gemma":[0.9995722,0.000025605555,0.00014875465,0.00007547497,0.000058368274,0.000119633325],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00016912089,0.0001850404,0.00019529277,0.0014803346,0.00024451356,0.0003206371,0.00020484881,0.00011039759,0.0007064369],"category_scores_gemma":[0.00032284035,0.00010834257,0.0001387336,0.00093367265,0.00018460405,0.0001693783,0.00051986077,0.00013030862,0.00029748215],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000060548828,0.000014888802,0.98072696,0.000014243324,0.00004038344,0.00010399716,0.00013947768,0.00019321151,0.009057801,0.000064942615,0.0006571134,0.008926346],"study_design_scores_gemma":[0.0000016878776,0.000007963042,0.99905473,0.0000015516172,0.000003510282,0.000054811742,0.00003999796,0.00015888053,0.0002524552,0.000005469469,0.00041793467,0.0000010808867],"about_ca_topic_score_codex":0.015963623,"about_ca_topic_score_gemma":0.035854865,"teacher_disagreement_score":0.015963623,"about_ca_system_score_codex":0.00032910125,"about_ca_system_score_gemma":0.0002119674,"threshold_uncertainty_score":0.03174138},"labels":[],"label_agreement":null},{"id":"W4414548078","doi":"10.3847/1538-4357/adfb64","title":"Metal-poor Star-forming Clumps in Cosmic Noon Galaxies: Evidence for Gas Inflow and Chemical Dilution Using JWST NIRISS","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Herzberg Institute of Astrophysics; York University; University of Toronto; Saint Mary's University","funders":"Natural Sciences and Engineering Research Council of Canada; Alliance de recherche numérique du Canada; Javna Agencija za Raziskovalno Dejavnost RS; Canadian Space Agency; Space Telescope Science Institute; Canadian Foundation for AIDS Research; Canarie; National Aeronautics and Space Administration; CSA Group","keywords":"Grism; Metallicity; Star formation; Galaxy; Line (geometry); Stars; James Webb Space Telescope","score_opus":0.020528209422635574,"score_gpt":0.2696249762875516,"score_spread":0.24909676686491602,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414548078","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99930096,0.00001805572,0.00012492499,0.000004325462,5.0629006e-7,0.0000028249258,0.00022969465,0.000015486145,0.0003032065],"genre_scores_gemma":[0.9988784,0.000013285431,0.00029654265,0.00000478447,0.0000018788055,0.0000023011792,0.00066065026,0.000006655153,0.00013542121],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99978536,0.00001662537,0.0000109659195,0.000057997153,0.0000779699,0.000051108073],"domain_scores_gemma":[0.9989336,0.00009517728,0.0003220346,0.00014637553,0.00018680624,0.00031601652],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032129377,0.00022194204,0.0002529964,0.0023620788,0.0004506529,0.00058669155,0.00041166594,0.00016831714,0.00060929975],"category_scores_gemma":[0.000862047,0.00015270557,0.00023242008,0.0012345957,0.00041941577,0.0002690566,0.00068843516,0.00019616094,0.00017602163],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00006274196,0.000016520888,0.9859211,0.000008020783,0.000030954398,0.000106810556,0.00026686155,0.00020828498,0.010990507,0.000062933424,0.000096160074,0.002229094],"study_design_scores_gemma":[6.9335493e-7,0.000005325552,0.99921536,7.653222e-7,0.0000029728471,0.00002545447,0.000056735997,0.00029522058,0.00032319844,0.0000073517294,0.00006534135,0.0000014992457],"about_ca_topic_score_codex":0.07105055,"about_ca_topic_score_gemma":0.14999165,"teacher_disagreement_score":0.07105055,"about_ca_system_score_codex":0.000611539,"about_ca_system_score_gemma":0.00026580115,"threshold_uncertainty_score":0.14127398},"labels":[],"label_agreement":null},{"id":"W4414553207","doi":"10.3847/1538-4357/adf8dd","title":"Resolution-corrected White Dwarf Gravitational Redshifts Validate Fifth-generation Sloan Digital Sky Survey Wavelength Calibration and Enable Accurate Mass–Radius Tests","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Leibniz-Gemeinschaft; National Astronomical Observatories, Chinese Academy of Sciences; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; University of Colorado Boulder; Leibniz-Institut für Astrophysik Potsdam; New Mexico State University; Nanjing University; Yale University; University of Toronto; École Polytechnique Fédérale de Lausanne; Space Telescope Science Institute; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; European Space Agency; Johns Hopkins University; Harvard University; China National Textile and Apparel Council; National Science Foundation; Yunnan University; California Institute of Technology; Ohio State University; Carnegie Institution of Washington; Smithsonian Astrophysical Observatory; Flatiron Health; Smithsonian Institution","keywords":"White dwarf; Sky; Redshift; Radial velocity; Calibration; Spectral resolution; Supernova; Spectral line","score_opus":0.017145205420787197,"score_gpt":0.24041228376299406,"score_spread":0.22326707834220685,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414553207","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9176823,0.00022173888,0.07225558,0.00014778378,0.000040771833,0.000028348437,0.0026123403,0.0017983597,0.005212731],"genre_scores_gemma":[0.98817015,0.00002348045,0.01028646,0.000032451484,0.000007961395,0.000007967851,0.0010628327,0.00009657596,0.0003120086],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99882,0.00027292792,0.00007712689,0.00031371124,0.00040038384,0.0001157166],"domain_scores_gemma":[0.99388003,0.0008288452,0.0016243205,0.0023026925,0.0011009891,0.0002630461],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.004568355,0.00034875766,0.00017331097,0.00087281025,0.0004262863,0.0007972707,0.0006176867,0.00032881115,0.0013659612],"category_scores_gemma":[0.010315614,0.00017893087,0.00030771492,0.00069320627,0.0003430857,0.0006389396,0.00080042327,0.000275027,0.0007835657],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00018827915,0.000101175996,0.8685098,0.00006305173,0.0002299835,0.000081989616,0.00027790054,0.05094707,0.016542194,0.008402733,0.0032769805,0.051378783],"study_design_scores_gemma":[0.000041596602,0.00009453625,0.7820861,0.000046484358,0.00007024587,0.00012230096,0.00017982718,0.17001404,0.033862468,0.004667219,0.008769065,0.000046242585],"about_ca_topic_score_codex":0.016737144,"about_ca_topic_score_gemma":0.017993703,"teacher_disagreement_score":0.016737144,"about_ca_system_score_codex":0.0009237019,"about_ca_system_score_gemma":0.000530852,"threshold_uncertainty_score":0.03327942},"labels":[],"label_agreement":null},{"id":"W4414553600","doi":"10.3847/1538-4357/adfcbf","title":"Stellar Obliquity Excitation via Disk-dispersal-driven Resonances in Binaries","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Binary number; Stars; Protoplanetary disk; Binary system; Stellar evolution; Phase (matter); Binary star; Star (game theory); Excitation","score_opus":0.008617200331369979,"score_gpt":0.25636451190650433,"score_spread":0.24774731157513435,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414553600","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9965379,0.000057576257,0.0022006428,0.000031623047,0.0000049387672,0.0000026512648,0.000017786742,0.000022239283,0.0011246586],"genre_scores_gemma":[0.9997621,0.000009067641,0.000096750744,0.0000029285793,0.0000011218659,5.1585585e-7,0.0000055197643,0.0000022314905,0.000119775825],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999409,0.000011412957,0.0000028666693,0.000015619149,0.000010339077,0.000018868954],"domain_scores_gemma":[0.99962413,0.00010292684,0.00010050746,0.000039562125,0.000031148084,0.000101745754],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00019536952,0.00016388968,0.00033544222,0.00035306494,0.0005986853,0.00084413914,0.00031782407,0.00034108426,0.0014251494],"category_scores_gemma":[0.00092658564,0.00016437296,0.00014421104,0.00019013592,0.00063771644,0.0006783126,0.001015568,0.000303847,0.00022437186],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007212888,0.00039219344,0.36784786,0.000150826,0.00018321637,0.0023508593,0.001340494,0.45618308,0.09510108,0.06064333,0.0011906499,0.01389515],"study_design_scores_gemma":[0.000060081446,0.00018401393,0.11003602,0.000017303752,0.00003236388,0.0005705623,0.0006169073,0.8576039,0.006142183,0.023494208,0.0011969488,0.000045419376],"about_ca_topic_score_codex":0.0045677936,"about_ca_topic_score_gemma":0.0034154577,"teacher_disagreement_score":0.0045677936,"about_ca_system_score_codex":0.00096389034,"about_ca_system_score_gemma":0.00021732341,"threshold_uncertainty_score":0.009082437},"labels":[],"label_agreement":null},{"id":"W4414588009","doi":"10.3847/1538-4357/adfbf6","title":"SQ-A: A Collision-triggered Starburst in the Intragroup Medium of Stephan’s Quintet","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Galaxy; Angular resolution (graph drawing); Data cube; Star formation; Kinematics; Displacement (psychology); Interstellar medium; Star (game theory)","score_opus":0.005850686900656725,"score_gpt":0.22474732852420595,"score_spread":0.21889664162354922,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414588009","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9974185,0.00003717339,0.0002928982,0.00008451613,0.000009076277,0.0000071019367,0.00007263691,0.000028193153,0.0020500077],"genre_scores_gemma":[0.9996183,0.000005393715,0.00012893602,0.000019459929,0.000003285254,0.0000017304412,0.00005255314,0.0000031849884,0.00016712552],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998939,0.0000107531505,0.0000029475996,0.000032006526,0.00002741188,0.000032945554],"domain_scores_gemma":[0.9993919,0.000080508726,0.00012698832,0.000066990106,0.00006412964,0.0002694408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018379281,0.00013526129,0.00014869634,0.0004246188,0.00080614234,0.00040422377,0.00039047372,0.00022754246,0.0027066306],"category_scores_gemma":[0.0005277107,0.00009595993,0.00012465502,0.00032684059,0.00042300014,0.00025863716,0.0009349046,0.0004034756,0.00021248664],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00089711434,0.00023423301,0.88337076,0.00007152934,0.0001379577,0.008061865,0.003361607,0.00088001724,0.07517096,0.0024134489,0.003295654,0.022104895],"study_design_scores_gemma":[0.00005643071,0.00036105266,0.976258,0.000014257702,0.00003193225,0.0030516787,0.0019375556,0.0032480895,0.0055761496,0.0016728982,0.0077606286,0.00003132998],"about_ca_topic_score_codex":0.0063504893,"about_ca_topic_score_gemma":0.012920491,"teacher_disagreement_score":0.0063504893,"about_ca_system_score_codex":0.00029413265,"about_ca_system_score_gemma":0.0001421415,"threshold_uncertainty_score":0.012627065},"labels":[],"label_agreement":null},{"id":"W4414617753","doi":"10.3847/1538-4357/adfb74","title":"Searching for Historical Extragalactic Optical Transients Associated with Fast Radio Bursts","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"H2020 European Research Council; Fonds de recherche du Québec – Nature et technologies; McGill Space Institute; University of Toronto; National Aeronautics and Space Administration; Canada Foundation for Innovation; Canadian Institute for Advanced Research; Research Corporation for Science Advancement; McGill University; Adolph C. and Mary Sprague Miller Institute for Basic Research in Science, University of California Berkeley; Gordon and Betty Moore Foundation; Natural Sciences and Engineering Research Council of Canada; Alfred P. Sloan Foundation; California Institute of Technology; David and Lucile Packard Foundation; National Science Foundation","keywords":"Redshift; Supernova; Ejecta; Observable; Observatory; Optical telescope; Fast radio burst; Transient (computer programming)","score_opus":0.011810781152325745,"score_gpt":0.2402979531998741,"score_spread":0.22848717204754834,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414617753","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99654883,0.00040938566,0.00051940244,0.000016814978,0.00000338311,0.000015386338,0.00067151885,0.000019555762,0.0017957217],"genre_scores_gemma":[0.99695516,0.00028122618,0.00079272635,0.000019683152,0.0000058121177,0.0000044119506,0.0014112643,0.000007002406,0.0005227356],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99972945,0.000016832986,0.00001275647,0.00007412725,0.0001049182,0.00006188864],"domain_scores_gemma":[0.9988192,0.00013065574,0.00048448256,0.00011971845,0.00023536525,0.00021049006],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00039380018,0.00018888207,0.00017157171,0.002959847,0.0006194542,0.0006322905,0.00037665854,0.00023564146,0.0015371968],"category_scores_gemma":[0.0012373303,0.00013022638,0.00022459125,0.001663335,0.0002765832,0.00028272165,0.00048396093,0.00016956897,0.0002935572],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004103235,0.000010955862,0.9865085,0.000023646118,0.00004076109,0.00017679084,0.000102287755,0.0001311572,0.0036488648,0.00007169003,0.00017090423,0.009073436],"study_design_scores_gemma":[0.0000012213177,0.000018247814,0.99800545,0.000009311072,0.00002279559,0.00025093343,0.000108086424,0.00018220677,0.00055716763,0.000016729284,0.00082442496,0.0000033169456],"about_ca_topic_score_codex":0.084018625,"about_ca_topic_score_gemma":0.194004,"teacher_disagreement_score":0.084018625,"about_ca_system_score_codex":0.00062558515,"about_ca_system_score_gemma":0.0006682115,"threshold_uncertainty_score":0.16705912},"labels":[],"label_agreement":null},{"id":"W4414795778","doi":"10.3847/1538-4357/ae060b","title":"A Search for Chemical Stratification and Magnetic Fields in Eight Field Blue Horizontal-branch Stars<sup>*</sup>","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Stars; Magnetic field; Spectral line; Stratification (seeds); Stellar atmosphere; Radial velocity; Field strength; Field (mathematics)","score_opus":0.008769977478827413,"score_gpt":0.23831183318467652,"score_spread":0.22954185570584912,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414795778","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991898,0.000036128004,0.00019417606,0.0000066495627,6.464019e-7,0.0000023453642,0.00019109965,0.00000876975,0.00037043125],"genre_scores_gemma":[0.9985245,0.000017146749,0.00061264343,0.000006570292,0.000002294472,0.0000018634103,0.00060742354,0.000005095779,0.00022252621],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999436,0.000006721166,0.0000036893841,0.000020811682,0.000015146872,0.0000100258985],"domain_scores_gemma":[0.99974805,0.0000417684,0.000060364222,0.000018035364,0.000070140355,0.00006159902],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00014968059,0.00013828177,0.00011719751,0.00085418974,0.00033937086,0.0002580273,0.00013404754,0.00016352722,0.0010346367],"category_scores_gemma":[0.00021247365,0.00008312099,0.00008774314,0.0005171435,0.00017241137,0.00011279921,0.00022792419,0.000103476894,0.00034989946],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013664844,0.00003610789,0.94416517,0.000016010192,0.000029029887,0.00006910617,0.00009273932,0.00029251058,0.047716886,0.00006368465,0.00011345972,0.0072687455],"study_design_scores_gemma":[0.000005821523,0.00004390435,0.9937263,0.0000014342294,0.000012359215,0.000076782606,0.00011253821,0.00075141015,0.004766091,0.000033009303,0.00046826038,0.0000020892567],"about_ca_topic_score_codex":0.004043831,"about_ca_topic_score_gemma":0.00707041,"teacher_disagreement_score":0.004043831,"about_ca_system_score_codex":0.00023822965,"about_ca_system_score_gemma":0.0001306124,"threshold_uncertainty_score":0.008040547},"labels":[],"label_agreement":null},{"id":"W4414845978","doi":"10.3847/1538-4357/adfddc","title":"The <i>z</i> ≳ 9 Galaxy UV Luminosity Function from the JWST Advanced Deep Extragalactic Survey: Insights into Early Galaxy Evolution and Reionization","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":32,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"Agencia Estatal de Investigación; European Commission; National Science Foundation; Royal Society; Science and Technology Facilities Council; National Research Foundation; Space Telescope Science Institute; Villum Fonden; Danmarks Grundforskningsfond; University of Arizona; University of California, Santa Cruz; Simons Foundation; Ministerio de Ciencia, Innovación y Universidades; National Aeronautics and Space Administration","keywords":"Reionization; Luminosity function; Galaxy; Population; Luminosity; Galaxy formation and evolution; Redshift","score_opus":0.006562189582029616,"score_gpt":0.20750310235474703,"score_spread":0.20094091277271742,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414845978","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99576265,0.000113537804,0.0008694041,0.0000428032,0.00000284074,0.0000036287042,0.0017715659,0.000064481974,0.0013691538],"genre_scores_gemma":[0.9962136,0.000045097393,0.00053716655,0.000017522756,0.000005110893,0.000002532289,0.002880435,0.000018184208,0.00028032323],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99986064,0.000014163898,0.000008098579,0.000033863173,0.000043405642,0.000039808965],"domain_scores_gemma":[0.9991246,0.00013426288,0.00033063916,0.0001046679,0.00012758562,0.00017826426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00042739895,0.0002300915,0.00022117312,0.0018071351,0.0001641734,0.0007071394,0.00032402133,0.00021543096,0.0014744884],"category_scores_gemma":[0.0009619449,0.0001224063,0.00043300758,0.0010620777,0.0001795617,0.00035075197,0.0005046928,0.00027079036,0.00068664935],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000029211255,0.00001234363,0.9883051,0.00001591542,0.000059110866,0.000055282813,0.000031365744,0.0012003732,0.0039998265,0.00017524598,0.0006035303,0.005512701],"study_design_scores_gemma":[0.0000013631998,0.0000075994685,0.9970656,0.0000027527417,0.000008825,0.000047217436,0.000019821931,0.0019629772,0.00043343107,0.000060424976,0.00038767493,0.0000023161538],"about_ca_topic_score_codex":0.0054793237,"about_ca_topic_score_gemma":0.005947536,"teacher_disagreement_score":0.0054793237,"about_ca_system_score_codex":0.00022892494,"about_ca_system_score_gemma":0.00011130569,"threshold_uncertainty_score":0.010894895},"labels":[],"label_agreement":null},{"id":"W4414846756","doi":"10.3847/1538-4357/adfdcc","title":"CHIME/FRB Outriggers: Design Overview","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Seismic and Structural Analysis of Tall Buildings","field":"Engineering","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Perimeter Institute; Banting Research Foundation; Canadian Institute for Theoretical Astrophysics; University of Toronto; Herzberg Institute of Astrophysics; McGill University; York University; Fonds de Recherche du Québec – Nature et Technologies; University of British Columbia","funders":"Gordon and Betty Moore Foundation","keywords":"Very-long-baseline interferometry; Galaxy; COSMIC cancer database; Interferometry; Baseline (sea); Calibration; Intensity mapping; Radio astronomy","score_opus":0.012934863157888382,"score_gpt":0.2284579788344743,"score_spread":0.2155231156765859,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414846756","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.1605043,0.0006560804,0.7143862,0.0011394273,0.00028434588,0.007085922,0.009692182,0.029174805,0.07707683],"genre_scores_gemma":[0.46266386,0.00042352264,0.4771465,0.0007216066,0.00006752164,0.0045706127,0.0056448416,0.0022035912,0.046557896],"study_design_codex":"design_other","study_design_gemma":"not_applicable","domain_scores_codex":[0.99921703,0.00011503635,0.000018742705,0.00012239043,0.00039152123,0.0001352491],"domain_scores_gemma":[0.99933076,0.000051111292,0.00004862602,0.00009723883,0.0003470937,0.00012517534],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0011110266,0.00093468104,0.00038764995,0.00068083784,0.0005884419,0.0010899917,0.0021792173,0.00061048236,0.0159301],"category_scores_gemma":[0.0010763048,0.00047890862,0.00029913397,0.0005147618,0.00041033403,0.00042960737,0.001014351,0.00047808734,0.004498602],"study_design_candidate":"not_applicable","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0038108835,0.0010543497,0.036017194,0.0014044394,0.00020663659,0.0010254174,0.00097230315,0.09100116,0.30684578,0.017290337,0.08042936,0.45994216],"study_design_scores_gemma":[0.0008634042,0.004853817,0.068866566,0.000218209,0.00023290557,0.00078069454,0.00090368645,0.23307386,0.11213773,0.003516704,0.57418454,0.00036792038],"about_ca_topic_score_codex":0.027519958,"about_ca_topic_score_gemma":0.041981634,"teacher_disagreement_score":0.027519958,"about_ca_system_score_codex":0.0016540635,"about_ca_system_score_gemma":0.001913957,"threshold_uncertainty_score":0.054719567},"labels":[],"label_agreement":null},{"id":"W4414879819","doi":"10.3847/1538-4357/ae04e4","title":"The Influence of Central Body Tides on Catastrophic Disruptions of Close-in Planetary Satellites","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Agence Nationale de la Recherche","keywords":"Scaling; Scaling law; Tidal force; Solar System; Celestial mechanics; Tidal power; Venus","score_opus":0.0046886123584424875,"score_gpt":0.2267909386566634,"score_spread":0.2221023262982209,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414879819","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96659935,0.00018687795,0.019235644,0.00065806607,0.000066114524,0.000029610741,0.00022256632,0.00013798544,0.0128637245],"genre_scores_gemma":[0.9978877,0.000060738068,0.00048982864,0.000025882995,0.000011181144,0.000013651379,0.000027446014,0.000020441383,0.0014631344],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99983335,0.000064388194,0.000006332943,0.00002422062,0.000024254088,0.00004749182],"domain_scores_gemma":[0.99861693,0.00049257436,0.0003778174,0.0000931369,0.00012157286,0.00029801193],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005773654,0.00057795126,0.00048619515,0.00047534678,0.0008037385,0.0013649631,0.00091004,0.0008745272,0.0027811711],"category_scores_gemma":[0.004412735,0.00026957912,0.0005999311,0.00025235774,0.0015433193,0.0009339231,0.0014281798,0.0007846028,0.00022893258],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009865471,0.00005872235,0.008083003,0.000028723438,0.000041844203,0.00045338838,0.00013899215,0.9621888,0.0012229439,0.024692073,0.00099224,0.002000612],"study_design_scores_gemma":[0.000020976597,0.00006672766,0.0018752521,0.0000062397617,0.000018186254,0.000045159883,0.00008399645,0.9893239,0.00024130759,0.007959256,0.00034495242,0.000013988677],"about_ca_topic_score_codex":0.01582794,"about_ca_topic_score_gemma":0.006880949,"teacher_disagreement_score":0.01582794,"about_ca_system_score_codex":0.0011926572,"about_ca_system_score_gemma":0.00052410405,"threshold_uncertainty_score":0.03147167},"labels":[],"label_agreement":null},{"id":"W4414980170","doi":"10.3847/1538-4357/adfa23","title":"Final Moments. III. Explosion Properties and Progenitor Constraints of CSM-interacting Type II Supernovae","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"Lawrence Berkeley National Laboratory; Planetary Science Division; Deutsches Elektronen-Synchrotron; University of California Observatories; Smithsonian Astrophysical Observatory; University of Illinois at Urbana-Champaign; Max-Planck-Institut für Astronomie; Agencia Nacional de Investigación y Desarrollo; Grand Équipement National De Calcul Intensif; Eötvös Loránd Tudományegyetem; Stockholms Universitet; Universitetet i Oslo; Max-Planck-Gesellschaft; Smithsonian Institution; John Templeton Foundation; National Natural Science Foundation of China; Queen's University; Canada Research Chairs; Gordon and Betty Moore Foundation; Queen's University Belfast; Science Mission Directorate; University of Toronto; National Centre for Supercomputing Applications; People's Government of Yunnan Province; National Central University; Villum Fonden; Los Alamos National Laboratory; University of Washington; Johns Hopkins University; National Science Foundation; European Commission; California Institute of Technology; Turun Yliopisto; Aarhus Universitet; Deutsche Forschungsgemeinschaft; Háskóli Íslands; Nuclear Safety and Security Commission; Australian Research Council; Space Telescope Science Institute; W. M. Keck Foundation; National Aeronautics and Space Administration; Natural Sciences and Engineering Research Council of Canada; Durham University","keywords":"Supernova; Ejecta; Spectral line; Plateau (mathematics); Light curve; Progenitor; Spectroscopy; Emission spectrum; Binary number","score_opus":0.029492466163683437,"score_gpt":0.254236740262942,"score_spread":0.22474427409925857,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4414980170","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99682057,0.00008237516,0.0008986069,0.0000065983168,0.0000016458268,0.0000044572294,0.00035509182,0.00002308862,0.0018075244],"genre_scores_gemma":[0.99854773,0.00001979759,0.00020357006,0.0000017544786,0.0000024322474,0.0000029550226,0.00085660524,0.0000060592897,0.0003591375],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998988,0.000008655964,0.0000109491775,0.000026541613,0.000028157101,0.00002690708],"domain_scores_gemma":[0.99897456,0.00026707002,0.00030489973,0.00009166894,0.0001584571,0.00020338575],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003576403,0.00012738002,0.00018220046,0.000650508,0.00017556887,0.000661514,0.00025183448,0.00012460904,0.002276331],"category_scores_gemma":[0.0018968623,0.000083601524,0.00019065532,0.0003038461,0.00013936989,0.00024763038,0.00029863018,0.00016276311,0.00047009432],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0009304819,0.00007668939,0.9415522,0.00003922353,0.00008138536,0.00040871996,0.00014475644,0.004293033,0.0308087,0.002368744,0.0002836348,0.019012377],"study_design_scores_gemma":[0.000008570723,0.00015779443,0.9869065,0.0000057971406,0.000014229739,0.00042488697,0.00008037354,0.00595466,0.0051692026,0.0004960371,0.00077368336,0.000008200734],"about_ca_topic_score_codex":0.0012742899,"about_ca_topic_score_gemma":0.0015712745,"teacher_disagreement_score":0.002276331,"about_ca_system_score_codex":0.00019466403,"about_ca_system_score_gemma":0.00010125634,"threshold_uncertainty_score":0.0076150894},"labels":[],"label_agreement":null},{"id":"W4415023853","doi":"10.3847/1538-4357/adfc58","title":"GWSkyNet-Multi. II. An Updated Machine Learning Model for Rapid Classification of Gravitational-wave Events","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval; Mila - Quebec Artificial Intelligence Institute; University of British Columbia; McGill University","funders":"Indo-US Science and Technology Forum; Canadian Institute for Advanced Research","keywords":"Neutron star; Event (particle physics); Binary number; Detector; Gravitational wave; Binary classification; Object (grammar); Compact star","score_opus":0.03596157508233139,"score_gpt":0.3525212968787809,"score_spread":0.31655972179644953,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415023853","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.27396294,0.0012759464,0.6566588,0.004489393,0.0008543637,0.00050697254,0.011849105,0.04053909,0.009863337],"genre_scores_gemma":[0.83169484,0.00029258739,0.14580116,0.0011194893,0.00021847425,0.0005611228,0.011334436,0.00069417205,0.0082835825],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9996686,0.000062467036,0.000018745794,0.0001496975,0.000056962046,0.000043590888],"domain_scores_gemma":[0.99892175,0.00054096105,0.00009286319,0.00015003313,0.0002177939,0.00007659509],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0014126255,0.0015602978,0.0007371925,0.00088090845,0.0003682091,0.0011726711,0.0031857511,0.0018192502,0.003954089],"category_scores_gemma":[0.0037210933,0.0006431334,0.00092605397,0.000429478,0.00049049605,0.001870148,0.0011406346,0.0026921583,0.0016188134],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00039702398,0.00024623136,0.008221939,0.00008287321,0.00011866433,0.00014308054,0.000064328684,0.8824359,0.001525206,0.0032161348,0.016313476,0.08723518],"study_design_scores_gemma":[0.000005067222,0.0000125686265,0.00012872372,0.0000034450059,0.0000039123124,0.0000049720993,0.000001848613,0.99841034,0.00023629943,0.0009272307,0.00026189163,0.0000036762344],"about_ca_topic_score_codex":0.015555598,"about_ca_topic_score_gemma":0.016117938,"teacher_disagreement_score":0.015555598,"about_ca_system_score_codex":0.0015210464,"about_ca_system_score_gemma":0.0011720714,"threshold_uncertainty_score":0.030930102},"labels":[],"label_agreement":null},{"id":"W4415043974","doi":"10.3847/1538-4357/ae032c","title":"Bondi-like Accretion Flow Dynamics: The Role of Gravitational Potential","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Accretion (finance); Angular momentum; Gravitational potential; Galaxy; Gravitation; Stellar mass; Specific relative angular momentum; Dark matter","score_opus":0.003807909541195789,"score_gpt":0.2158905415110006,"score_spread":0.2120826319698048,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415043974","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92951643,0.0010976109,0.046857152,0.0010141159,0.0001002813,0.000041392992,0.00010842157,0.0001892098,0.021075334],"genre_scores_gemma":[0.99679273,0.00023547019,0.0021079932,0.000036556783,0.00003371863,0.000009395391,0.000024706134,0.000020899923,0.0007385635],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992406,0.000029472432,0.0000026772213,0.000014232202,0.0000120701925,0.00001758237],"domain_scores_gemma":[0.99967766,0.000084826315,0.00009952911,0.000025053863,0.00003456925,0.00007839789],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035365956,0.00039235677,0.00042666154,0.00041640416,0.0004682089,0.0013524507,0.0005856831,0.0006441508,0.0012824641],"category_scores_gemma":[0.0017238666,0.00023224221,0.0003289011,0.00022230927,0.0011790369,0.0010942458,0.0007523112,0.0004947454,0.00014958472],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023519662,0.00010131834,0.017644167,0.00013183388,0.000095958305,0.000676561,0.00036891762,0.4738391,0.023698583,0.47018975,0.0021868064,0.0108318785],"study_design_scores_gemma":[0.000017429364,0.00001662625,0.0032321187,0.000009504237,0.000007461312,0.000059792288,0.000036483532,0.9728703,0.0004814052,0.022764085,0.00048845017,0.000016399157],"about_ca_topic_score_codex":0.0050362283,"about_ca_topic_score_gemma":0.0012878972,"teacher_disagreement_score":0.0050362283,"about_ca_system_score_codex":0.00080548547,"about_ca_system_score_gemma":0.000382437,"threshold_uncertainty_score":0.010013819},"labels":[],"label_agreement":null},{"id":"W4415254768","doi":"10.3847/1538-4357/ae07ce","title":"The Dark Matter Content of Milky Way Dwarf Spheroidal Galaxies: Draco, Sextans, and Ursa Minor","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Division of Astronomical Sciences; Higher Education Discipline Innovation Project; Science and Technology Facilities Council; Agencia Estatal de Investigación; Office of Science; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; National Natural Science Foundation of China; National Science Foundation; Shanghai Jiao Tong University; National Energy Research Scientific Computing Center; Gordon and Betty Moore Foundation; U.S. Department of Energy","keywords":"Milky Way; Dark matter; Galaxy; Stars; Local Group; Velocity dispersion; Dwarf spheroidal galaxy; Dwarf galaxy","score_opus":0.009876576888860842,"score_gpt":0.2182380106566691,"score_spread":0.20836143376780825,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415254768","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9995561,0.000032534248,0.000018627248,0.000008413585,3.7952938e-7,7.031694e-7,0.00014867583,0.000006148974,0.0002283973],"genre_scores_gemma":[0.9993563,0.00001690934,0.000029531728,0.0000038418952,0.0000010931581,8.4006757e-7,0.0004871574,0.0000021462372,0.00010220946],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999286,0.000008698923,0.0000052420137,0.00002842711,0.000012873414,0.000016152853],"domain_scores_gemma":[0.9995561,0.000054393025,0.00015707086,0.000058913483,0.00006359384,0.00010991802],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017780904,0.00016903157,0.00014392681,0.0009136078,0.00017864327,0.00042288663,0.00022161302,0.0001431236,0.00089476956],"category_scores_gemma":[0.00071289664,0.00008241193,0.0001753691,0.00042254757,0.00029231497,0.00018321017,0.00035006728,0.00008876312,0.00024363182],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004872356,0.0000075448515,0.99559635,0.000005083192,0.000033398675,0.000038702594,0.00015785109,0.00027585885,0.0017978367,0.0001275779,0.0001371502,0.001773946],"study_design_scores_gemma":[0.0000022819884,0.000005380595,0.9989648,0.0000013788629,0.0000064083006,0.000026856655,0.00007493639,0.0005897439,0.00016456403,0.000031418887,0.00013077978,0.000001492084],"about_ca_topic_score_codex":0.01498962,"about_ca_topic_score_gemma":0.013844209,"teacher_disagreement_score":0.01498962,"about_ca_system_score_codex":0.0003700545,"about_ca_system_score_gemma":0.00009506644,"threshold_uncertainty_score":0.029804707},"labels":[],"label_agreement":null},{"id":"W4415303463","doi":"10.3847/1538-4357/adf844","title":"Morphology of 35 Repeating Fast Radio Burst Sources at Microsecond Time Scales with CHIME/FRB","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":8,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Smithsonian Astrophysical Observatory; University of Toronto","keywords":"Microsecond; Scattering; Dispersion (optics); Temporal resolution; Measure (data warehouse); Spectral shape analysis; Intensity (physics); Spectral line","score_opus":0.004791219082692477,"score_gpt":0.2675531183927232,"score_spread":0.26276189931003074,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415303463","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9987784,0.00013037809,0.00020627127,0.000012161692,0.0000017327939,0.000008364046,0.00032881869,0.000022621747,0.00051120494],"genre_scores_gemma":[0.998145,0.00006291331,0.00059655204,0.00001086304,0.000003437803,0.0000066335756,0.0008656444,0.00001530077,0.00029368905],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998821,0.000005251106,0.000009141294,0.000031765314,0.000040085182,0.000031615655],"domain_scores_gemma":[0.99932265,0.000091503454,0.0002603861,0.00007885789,0.000106790416,0.00013980836],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00018173078,0.00016409812,0.00020975346,0.0019188921,0.00040669655,0.0005123753,0.00032251366,0.0002041426,0.0010280062],"category_scores_gemma":[0.000762296,0.00017305388,0.00017659555,0.0015160425,0.00025313755,0.00017529838,0.0005950329,0.00015209842,0.00023652632],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038453084,0.000043193635,0.8497797,0.000042736894,0.00011243651,0.0011175603,0.0012850845,0.00035418948,0.112155005,0.00011647099,0.00035835002,0.03425079],"study_design_scores_gemma":[0.000001909695,0.000013628458,0.99844164,0.000001818322,0.0000070942538,0.00030939642,0.00007421754,0.00010054771,0.00078167033,0.000015674834,0.0002487531,0.0000035497105],"about_ca_topic_score_codex":0.011861898,"about_ca_topic_score_gemma":0.012472926,"teacher_disagreement_score":0.011861898,"about_ca_system_score_codex":0.00037021452,"about_ca_system_score_gemma":0.000116694675,"threshold_uncertainty_score":0.023585677},"labels":[],"label_agreement":null},{"id":"W4415374642","doi":"10.3847/1538-4357/ae06a4","title":"<scp>Aeos</scp>: The Impact of Population III Initial Mass Function and Star-by-star Models in Galaxy Simulations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria","funders":"National Aeronautics and Space Administration","keywords":"Galaxy; Population; Initial mass function; Stars; Galaxy formation and evolution; Stellar population; Star formation","score_opus":0.012596446743114,"score_gpt":0.2592398400187825,"score_spread":0.24664339327566848,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415374642","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.92598075,0.00031427183,0.010067465,0.0026449277,0.00032020677,0.000117652315,0.010907129,0.0039450554,0.045702476],"genre_scores_gemma":[0.98161453,0.00020120415,0.008906499,0.0005248281,0.00007404555,0.00015538749,0.0042455653,0.0014909043,0.002786965],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999537,0.00020518807,0.000025593421,0.000045757068,0.0001113421,0.00007515005],"domain_scores_gemma":[0.9936913,0.003956262,0.00033638123,0.00051567826,0.0008699387,0.000630403],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012403086,0.00062174886,0.0008845208,0.0005770813,0.0006787336,0.0011918702,0.0015038362,0.00091100903,0.011227524],"category_scores_gemma":[0.006272788,0.00034220144,0.00080732664,0.00083508156,0.0006055205,0.00092465075,0.0008422606,0.0014769778,0.00095589575],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000613317,0.00053236104,0.022729227,0.00019827449,0.000270503,0.000421482,0.00019155978,0.9247799,0.0036366032,0.011193479,0.027880944,0.0075523825],"study_design_scores_gemma":[0.00023092392,0.000118665106,0.0046741203,0.000035424884,0.00003343288,0.00002932846,0.00009755254,0.9852276,0.0032923324,0.003031126,0.0031975557,0.00003201513],"about_ca_topic_score_codex":0.0216953,"about_ca_topic_score_gemma":0.014296112,"teacher_disagreement_score":0.0216953,"about_ca_system_score_codex":0.0008966928,"about_ca_system_score_gemma":0.0008358191,"threshold_uncertainty_score":0.043138027},"labels":[],"label_agreement":null},{"id":"W4415421528","doi":"10.3847/1538-4357/adf217","title":"Late-time Evolution of Magnetized Disks in Tidal Disruption Events","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Azrieli Foundation; Israel Science Foundation; United States - Israel Binational Science Foundation","keywords":"Supermassive black hole; Accretion disc; Accretion (finance); Viscosity; Quasiperiodic function; Magnetic field; Radiation pressure","score_opus":0.00634928233778801,"score_gpt":0.23775453057045268,"score_spread":0.23140524823266467,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415421528","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99855465,0.0001001255,0.00083596417,0.00003128322,0.0000033197523,0.0000026016362,0.00010180627,0.000019645231,0.00035056032],"genre_scores_gemma":[0.99968565,0.000016735745,0.00013235245,0.000003392895,0.0000023611326,0.0000010831372,0.000069935864,0.0000029278306,0.000085620646],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99994206,0.000009033029,0.0000031642212,0.00002249956,0.000007950982,0.000015138877],"domain_scores_gemma":[0.999458,0.00012499909,0.00019569181,0.000034709305,0.00006323757,0.00012332502],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028917522,0.00019775685,0.00018095304,0.0008419088,0.00028657334,0.0006820299,0.00034780492,0.00043309777,0.00086127355],"category_scores_gemma":[0.0013879694,0.00014320017,0.00025591662,0.0004016652,0.0002629338,0.0005544265,0.00039977176,0.00028741694,0.00012959463],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0005857739,0.00016331264,0.808798,0.000077093784,0.00020574898,0.0020433275,0.00066146645,0.115626186,0.049503352,0.0069241766,0.0008598445,0.014551653],"study_design_scores_gemma":[0.00003128359,0.00015005302,0.6462318,0.00002134414,0.000047997302,0.00048183478,0.00030937785,0.34333432,0.0049218587,0.0031642185,0.001249353,0.000056540728],"about_ca_topic_score_codex":0.0021795947,"about_ca_topic_score_gemma":0.0013346423,"teacher_disagreement_score":0.0021795947,"about_ca_system_score_codex":0.00053853536,"about_ca_system_score_gemma":0.00008884645,"threshold_uncertainty_score":0.0043338537},"labels":[],"label_agreement":null},{"id":"W4415430692","doi":"10.3847/1538-4357/ae0ace","title":"Tracing Planetary Accretion in a 3 Gyr old Hydrogen-rich White Dwarf: The Extremely Polluted Atmosphere of LSPM J0207+3331","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Centre for Research in Astrophysics of Québec; HEC Montréal","funders":"","keywords":"White dwarf; Accretion (finance); Photosphere; Atmosphere (unit); Line (geometry); Stellar atmosphere; Infrared excess; Spectral line; Opacity","score_opus":0.00923328612725577,"score_gpt":0.21859693382839576,"score_spread":0.20936364770114,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415430692","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994535,0.00002046842,0.000119872755,0.000010376511,0.0000019360461,0.0000022693594,0.000120673365,0.00001738115,0.0002535812],"genre_scores_gemma":[0.9992908,0.000012811697,0.0002425884,0.000012409579,0.000004384342,0.0000029909795,0.00031073694,0.0000068137865,0.00011634525],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995136,0.0000049537366,0.0000015305372,0.000013660172,0.000012447043,0.000016062218],"domain_scores_gemma":[0.9998765,0.000015996662,0.000023850258,0.000013237589,0.000019599334,0.000050817314],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001689191,0.00022312686,0.00027680397,0.00050406944,0.0005013518,0.0002895333,0.00026307348,0.0003660858,0.00037499575],"category_scores_gemma":[0.00018202177,0.0001457462,0.00018633607,0.00026685366,0.00019483265,0.00014926656,0.000458456,0.00027031184,0.00025358348],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024391827,0.00011572175,0.86702275,0.000040082745,0.00007825348,0.0029601762,0.0009407722,0.0011777437,0.12034295,0.00017230523,0.0005762208,0.006329088],"study_design_scores_gemma":[0.0000049670352,0.00010441282,0.9906476,0.000003599016,0.000021457256,0.0004819416,0.00022929357,0.0033263708,0.0043457844,0.00004227814,0.0007858208,0.000006467741],"about_ca_topic_score_codex":0.004909793,"about_ca_topic_score_gemma":0.00824179,"teacher_disagreement_score":0.004909793,"about_ca_system_score_codex":0.00030993222,"about_ca_system_score_gemma":0.00014527002,"threshold_uncertainty_score":0.009762406},"labels":[],"label_agreement":null},{"id":"W4415455320","doi":"10.3847/1538-4357/ae003d","title":"Do White Dwarfs Sample Water-rich Planetary Material?","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université de Montréal; Montreal Clinical Research Institute","funders":"National Aeronautics and Space Administration","keywords":"White dwarf; Accretion (finance); Population; Black dwarf; White (mutation); Atmosphere (unit); Range (aeronautics); Massive compact halo object","score_opus":0.006286828797706834,"score_gpt":0.20890353259703714,"score_spread":0.2026167037993303,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415455320","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99883217,0.000106887535,0.00043827962,0.0000163847,0.0000028260738,0.0000032582707,0.00012925599,0.000014617312,0.00045634888],"genre_scores_gemma":[0.9995757,0.00003066132,0.00012733683,0.000018228237,0.000003793955,0.0000013879331,0.00014341365,0.00000650065,0.00009309642],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99958104,0.000043791482,0.00004263857,0.00016605473,0.00009108494,0.00007542555],"domain_scores_gemma":[0.998801,0.00022686762,0.0004582686,0.00018283262,0.000182033,0.00014893929],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005644318,0.00020183825,0.00040911147,0.001136229,0.00046736415,0.00094671885,0.00032474223,0.00029722304,0.00070839433],"category_scores_gemma":[0.0015632035,0.0001738474,0.00017300273,0.0008093012,0.00069742,0.00055651413,0.00068626954,0.00014331588,0.000288437],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0000813379,0.000007907216,0.98458976,0.000014855612,0.000054800243,0.000042741118,0.00026504812,0.00008460498,0.01192807,0.00009356749,0.000069123336,0.00276825],"study_design_scores_gemma":[0.0000038224985,0.000027335038,0.99610066,0.0000029361322,0.000016766031,0.000099434365,0.00032420244,0.00036751162,0.002419097,0.00019654725,0.00043840086,0.0000033061033],"about_ca_topic_score_codex":0.003472205,"about_ca_topic_score_gemma":0.005850518,"teacher_disagreement_score":0.003472205,"about_ca_system_score_codex":0.00026844803,"about_ca_system_score_gemma":0.0001270949,"threshold_uncertainty_score":0.006904006},"labels":[],"label_agreement":null},{"id":"W4415461617","doi":"10.3847/1538-4357/ae0471","title":"Environment of SDSS Quasars at <i>z</i> = 0.4–1.0 Explored by Subaru HSC","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; Max-Planck-Gesellschaft; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; Eötvös Loránd Tudományegyetem; Academia Sinica; Space Telescope Science Institute; Los Alamos National Laboratory; Johns Hopkins University; Princeton University; National Central University; Queen's University Belfast; Gordon and Betty Moore Foundation; Japan Society for the Promotion of Science; National Aeronautics and Space Administration; Durham University; Japan Science and Technology Agency; Smithsonian Institution; National Science Foundation","keywords":"Quasar; Supermassive black hole; Galaxy; Sky; Redshift; Active galactic nucleus; Galaxy formation and evolution; OVV quasar","score_opus":0.005689726054399542,"score_gpt":0.19518021151629827,"score_spread":0.18949048546189873,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415461617","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994504,0.000027472877,0.000053257565,0.000010721088,5.4781276e-7,0.0000010088357,0.00019260606,0.000004799566,0.0002591237],"genre_scores_gemma":[0.99951077,0.000015308911,0.00007274743,0.0000060407506,0.0000018783103,0.0000010081945,0.00033600253,0.0000015178894,0.00005467034],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99985456,0.000032839143,0.0000067120995,0.000037435013,0.000028115743,0.000040325096],"domain_scores_gemma":[0.99951994,0.00006258164,0.00018774661,0.000038192546,0.000075448144,0.00011609547],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00029558715,0.00013291501,0.00025173917,0.0011119313,0.0003107669,0.000554217,0.00021214552,0.00011929867,0.0007009295],"category_scores_gemma":[0.00038494015,0.00012694,0.00019512935,0.00094428967,0.00024751353,0.0002591318,0.0005436015,0.00012799952,0.00015338957],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00004612654,0.000018930077,0.9935638,0.0000069659195,0.00003687404,0.00006768682,0.00012435332,0.0003794141,0.0038575581,0.00009297179,0.00015255963,0.0016528628],"study_design_scores_gemma":[0.0000010276594,0.000010173082,0.9992625,7.1929486e-7,0.0000055757023,0.000018891089,0.0000903942,0.0003363817,0.00017610907,0.0000149535335,0.00008163016,0.0000016177315],"about_ca_topic_score_codex":0.011648096,"about_ca_topic_score_gemma":0.013384239,"teacher_disagreement_score":0.011648096,"about_ca_system_score_codex":0.00023533567,"about_ca_system_score_gemma":0.0001514846,"threshold_uncertainty_score":0.023160577},"labels":[],"label_agreement":null},{"id":"W4415607438","doi":"10.3847/1538-4357/ae045c","title":"The Aromatic Infrared Bands around the Wolf–Rayet Binary WR 140 Revealed by JWST","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; Université de Montréal; Centre for Research in Astrophysics of Québec","funders":"National Astronomical Observatory of Japan","keywords":"Infrared; Stars; Shell (structure); Spectral line; Circumstellar dust; Wavelength; Infrared spectroscopy; Spitzer Space Telescope; James Webb Space Telescope","score_opus":0.006215799345046243,"score_gpt":0.23509520803240308,"score_spread":0.22887940868735684,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415607438","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9992119,0.00005383423,0.000105748455,0.0000061532496,0.0000017007231,0.0000011817833,0.00006364691,0.000012445137,0.00054339465],"genre_scores_gemma":[0.9994116,0.000016948408,0.00016396215,0.0000089343785,0.000004314705,0.0000013259912,0.00023885879,0.0000055436108,0.0001485785],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999434,0.000002927312,0.0000022889121,0.000017969965,0.000017933313,0.000015614392],"domain_scores_gemma":[0.9998293,0.000013792279,0.000065406886,0.000014568411,0.000025408706,0.000051544892],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00010240068,0.00015962598,0.00017642791,0.00074244314,0.00024394724,0.00032364592,0.00020061262,0.00017447029,0.00091141666],"category_scores_gemma":[0.00017664726,0.00012497256,0.00013340308,0.00039158703,0.00016124602,0.00020742,0.0003819371,0.00023384622,0.00021274247],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006325676,0.000100497055,0.44943744,0.0000562557,0.00014359175,0.0014471108,0.0004339782,0.00034809476,0.53013825,0.00029155763,0.00036384523,0.016606865],"study_design_scores_gemma":[0.0000071821087,0.000058051795,0.9923356,0.0000029192822,0.000017455879,0.000308598,0.00009811373,0.00034748018,0.0060812416,0.000040249208,0.0006995338,0.0000036415277],"about_ca_topic_score_codex":0.0009146198,"about_ca_topic_score_gemma":0.0012242426,"teacher_disagreement_score":0.0009146198,"about_ca_system_score_codex":0.0001448237,"about_ca_system_score_gemma":0.000043815857,"threshold_uncertainty_score":0.0030489564},"labels":[],"label_agreement":null},{"id":"W4415655298","doi":"10.3847/1538-4357/ae04df","title":"Balmer Absorption in Iron Low-ionization Broad Absorption Line Quasars","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Brookhaven National Laboratory; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Gesellschaft; Chinese Academy of Sciences; York University; Fermilab; National Science Foundation; Case Western Reserve University; UK Research and Innovation; Universität Basel; Carnegie Mellon University; University of Pittsburgh; Los Alamos National Laboratory; College of Engineering, Michigan State University; Princeton University; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Harvard University; Ohio State University; New Mexico State University; University of Portsmouth; Yale University; Drexel University; Vanderbilt University; University of Oklahoma; National Aeronautics and Space Administration; U.S. Naval Observatory; U.S. Department of Energy","keywords":"Balmer series; Quasar; Outflow; Absorption (acoustics); Spectral line; Absorption spectroscopy","score_opus":0.005922439218581206,"score_gpt":0.224213242774006,"score_spread":0.2182908035554248,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415655298","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9994925,0.000050260984,0.000083713,0.000004753523,6.540462e-7,0.0000022291513,0.000060444814,0.0000036062813,0.00030184933],"genre_scores_gemma":[0.9996258,0.000020599737,0.00009950393,0.000007938893,0.0000016919134,0.0000022513013,0.00012882562,0.0000013938685,0.0001120724],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.999833,0.00001959209,0.000014275069,0.000051442545,0.000034609162,0.000047041754],"domain_scores_gemma":[0.9992175,0.000120628196,0.0003583153,0.000045306202,0.00010197505,0.0001562594],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00032292688,0.00023104998,0.00022091705,0.0020009845,0.0004051049,0.0005513051,0.00022144847,0.00024273545,0.0016472137],"category_scores_gemma":[0.000877498,0.000116118485,0.0001093114,0.0007093428,0.0004032339,0.00029592606,0.00045517206,0.00020627669,0.00025447234],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000033730787,0.000023720986,0.99135965,0.000005788052,0.000008657297,0.000050776333,0.000111160916,0.000024438077,0.006604486,0.00003241044,0.000022411208,0.0017226309],"study_design_scores_gemma":[0.0000012792523,0.000028476981,0.9991584,0.0000023734585,0.0000033584672,0.00010534992,0.000105550556,0.000059622984,0.00039907635,0.000019049365,0.00011638143,0.000001182198],"about_ca_topic_score_codex":0.0021569908,"about_ca_topic_score_gemma":0.0035257565,"teacher_disagreement_score":0.0021569908,"about_ca_system_score_codex":0.00021065859,"about_ca_system_score_gemma":0.00007441154,"threshold_uncertainty_score":0.0055104494},"labels":[],"label_agreement":null},{"id":"W4415686868","doi":"10.3847/1538-4357/ae08b5","title":"Lunar Highland Preserves Meteoritic-iron-rich Materials in the Earth–Moon System","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Planetary Science and Exploration","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Geology of the Moon; Meteorite; Impact crater; Earth (classical element); Lunar soil; Regolith; Achondrite; Chondrite","score_opus":0.009444604132881604,"score_gpt":0.22407429931003736,"score_spread":0.21462969517715574,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415686868","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99963,0.000056470573,0.00001655206,0.0000027557292,2.7448715e-7,6.5105297e-7,0.00006652698,0.0000021345372,0.00022478976],"genre_scores_gemma":[0.9997029,0.00003243647,0.000028548286,0.0000020629132,6.26763e-7,5.4617783e-7,0.00009139487,0.0000010557685,0.0001405224],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99994624,0.000003669575,0.0000036588958,0.000015199988,0.000010689185,0.00002048408],"domain_scores_gemma":[0.99989116,0.000008294633,0.000049924864,0.0000072713133,0.000019807634,0.000023488788],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000067681445,0.00010818895,0.00018751364,0.0013796745,0.0004465224,0.00048787825,0.00008549369,0.00008113497,0.0010608648],"category_scores_gemma":[0.00013638637,0.000091429894,0.00007140989,0.0007687243,0.00031885685,0.00014615062,0.00030347903,0.00009344619,0.00013559342],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00019896594,0.000016110116,0.88313437,0.000036916466,0.000043753225,0.00041204764,0.0006617802,0.0001258903,0.10662342,0.000072220224,0.00007875745,0.008595763],"study_design_scores_gemma":[5.6724406e-7,0.0000077368395,0.9985531,0.0000014296708,0.0000034573545,0.0000870158,0.00016820291,0.000033948687,0.0009469065,0.0000063867988,0.00019045969,7.446511e-7],"about_ca_topic_score_codex":0.013953342,"about_ca_topic_score_gemma":0.031680483,"teacher_disagreement_score":0.013953342,"about_ca_system_score_codex":0.00026532362,"about_ca_system_score_gemma":0.00014430995,"threshold_uncertainty_score":0.027744234},"labels":[],"label_agreement":null},{"id":"W4415687287","doi":"10.3847/1538-4357/ae0623","title":"The Dipole Instability in Gravitational <i>N</i> -body Systems: A Natural Explanation for Lopsidedness and Off-centered Nuclei in Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Perimeter Institute","funders":"","keywords":"Instability; Dipole; Inflection point; Quadrupole; Angular momentum; Isotropy; Soliton; Halo","score_opus":0.008704625512074276,"score_gpt":0.25327095539535005,"score_spread":0.24456632988327578,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415687287","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9868182,0.000058478407,0.008856787,0.00027308438,0.0000073373362,0.000011274153,0.000017828479,0.000076903605,0.0038801816],"genre_scores_gemma":[0.9995154,0.000007702884,0.00032325913,0.000012993669,0.0000018435971,0.0000018982031,0.0000035683343,0.0000037939649,0.00012960086],"study_design_codex":"simulation_or_modeling","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.99997175,0.0000062864174,0.0000010888584,0.0000044681397,0.000005798023,0.000010586314],"domain_scores_gemma":[0.9998574,0.000035677982,0.00003884352,0.000017950608,0.00001327063,0.00003679118],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015078521,0.00014391253,0.00016206728,0.00028230334,0.00043681025,0.0004797234,0.0004597744,0.0004132373,0.0010435804],"category_scores_gemma":[0.0005350441,0.0000982758,0.00020261202,0.00009439309,0.000996442,0.00041468718,0.0004553847,0.00025045336,0.000098534045],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003192901,0.00018522982,0.12209144,0.0001024069,0.00011058253,0.0022932086,0.0019889304,0.5370564,0.11397196,0.20432428,0.0023612995,0.015195037],"study_design_scores_gemma":[0.000051531373,0.00010413705,0.026782742,0.0000120288205,0.000009065311,0.0003296151,0.00038826192,0.9177024,0.004590472,0.048815705,0.0011850289,0.000029085892],"about_ca_topic_score_codex":0.003014862,"about_ca_topic_score_gemma":0.0016518586,"teacher_disagreement_score":0.003014862,"about_ca_system_score_codex":0.0006435464,"about_ca_system_score_gemma":0.00019985085,"threshold_uncertainty_score":0.005994618},"labels":[],"label_agreement":null},{"id":"W4415688736","doi":"10.3847/1538-4357/ae0922","title":"Calcium Excess in Novae: Beyond Nuclear Physics Uncertainties","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Victoria; TRIUMF","funders":"","keywords":"Nova (rocket); Abundance (ecology); Nucleosynthesis; Nuclear reaction; Monte Carlo method; Isotopes of calcium","score_opus":0.01530803446539009,"score_gpt":0.25825443476443666,"score_spread":0.24294640029904657,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415688736","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99516946,0.0004877425,0.0014452499,0.00009245828,0.0000085375605,0.000004321281,0.00031778307,0.000028979228,0.0024455052],"genre_scores_gemma":[0.999401,0.000056154837,0.0002542876,0.000014024832,0.0000025800866,0.0000011027607,0.00012721858,0.0000072096086,0.00013644905],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9997584,0.000035651723,0.000018748031,0.0000967599,0.00006488697,0.00002565161],"domain_scores_gemma":[0.99825567,0.00065719255,0.0005388886,0.00019676819,0.00020569707,0.00014571482],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008584293,0.00026873304,0.0003985408,0.0011169517,0.00051560614,0.0012566211,0.0004871491,0.0005600503,0.0013727243],"category_scores_gemma":[0.004304981,0.00022976157,0.00037223153,0.0006823481,0.0006638881,0.0006927272,0.0010069348,0.0002932839,0.00021664979],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00024923656,0.000016968752,0.9560737,0.00009118237,0.00019167196,0.00040050823,0.00012617883,0.019056369,0.014188671,0.0020362553,0.00019134796,0.0073779514],"study_design_scores_gemma":[0.000012025497,0.000046690922,0.95495987,0.00002864013,0.000037241443,0.00039864166,0.0001718716,0.036175244,0.0035343252,0.002980627,0.0016281371,0.00002668113],"about_ca_topic_score_codex":0.005903117,"about_ca_topic_score_gemma":0.006107323,"teacher_disagreement_score":0.005903117,"about_ca_system_score_codex":0.0007179008,"about_ca_system_score_gemma":0.00015492488,"threshold_uncertainty_score":0.011737525},"labels":[],"label_agreement":null},{"id":"W4415746897","doi":"10.3847/1538-4357/ae0335","title":"Hubble Space Telescope Deep Upper Limits Rule out a Surviving Massive Binary Companion to the Type Ic Supernova 2012fh","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Space Telescope Science Institute","keywords":"Supernova; Binary number; Luminosity; Hubble space telescope; Population; Hubble Deep Field; Diagram; Binary Independence Model; Stellar evolution","score_opus":0.013126154372634397,"score_gpt":0.2517556734992903,"score_spread":0.2386295191266559,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415746897","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.96997166,0.00035500084,0.003513567,0.00012042341,0.000045883447,0.000023899123,0.0016674169,0.0003072279,0.023994854],"genre_scores_gemma":[0.9939704,0.000094348485,0.0021120575,0.000081776416,0.000034662527,0.0000059003746,0.0018371771,0.00002014981,0.0018434437],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987686,0.0000072392563,0.000010821286,0.00003320522,0.000038012575,0.00003386414],"domain_scores_gemma":[0.9992472,0.00009698972,0.00022570688,0.000113300164,0.00009900157,0.00021788085],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003967711,0.00028094876,0.00023839164,0.0009749194,0.00043379312,0.0009761345,0.0003006026,0.0004053353,0.007377916],"category_scores_gemma":[0.0012532007,0.00015265374,0.00028452635,0.00029351524,0.00028904868,0.00034567065,0.0003850789,0.00026719173,0.0013732472],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001737345,0.00007140325,0.93339735,0.000061943574,0.000067793306,0.000770983,0.00018947414,0.0007402259,0.030110143,0.0023742681,0.003623802,0.028418792],"study_design_scores_gemma":[0.000008672264,0.00004394724,0.9856328,0.000033015876,0.000016432974,0.00092095055,0.00012250403,0.0020004576,0.004058852,0.0011413862,0.0060129627,0.000008008747],"about_ca_topic_score_codex":0.004781365,"about_ca_topic_score_gemma":0.010614972,"teacher_disagreement_score":0.007377916,"about_ca_system_score_codex":0.00033021063,"about_ca_system_score_gemma":0.00017492572,"threshold_uncertainty_score":0.024681628},"labels":[],"label_agreement":null},{"id":"W4415902319","doi":"10.3847/1538-4357/ae093b","title":"Investigating the Sightline of a Highly Scattered Fast Radio Burst through a Cosmic Sheet Structure in the Local Universe","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":3,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Nederlandse Organisatie voor Wetenschappelijk Onderzoek; Canada Foundation for Innovation; National Aeronautics and Space Administration","keywords":"Galaxy; Scattering; Fast radio burst; Universe; Mean free path; COSMIC cancer database; Structure formation; Measure (data warehouse)","score_opus":0.010865051668019612,"score_gpt":0.290994131995686,"score_spread":0.2801290803276664,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415902319","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9973877,0.000023379536,0.00019038696,0.000022290196,9.175658e-7,0.000002823042,0.0004940488,0.000014729801,0.0018636335],"genre_scores_gemma":[0.9984339,0.000021174195,0.00032724862,0.000011575391,0.000002198907,0.0000022112465,0.00060759933,0.0000057815637,0.0005884852],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99995923,0.000005897117,0.0000016388607,0.000010869239,0.000010812027,0.000011438981],"domain_scores_gemma":[0.9995616,0.000066031134,0.00013647696,0.000038498616,0.000056653884,0.00014084196],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011691533,0.000077825,0.000066218454,0.00074045657,0.0002980357,0.00034574675,0.00012755151,0.00012896751,0.0024536033],"category_scores_gemma":[0.00053270994,0.00005203964,0.00006568012,0.0005789999,0.0001224461,0.00019087378,0.000247544,0.00011057575,0.0003660762],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059608836,0.000020904605,0.98302746,0.000012536358,0.000018557474,0.00017524305,0.0005931071,0.00046205148,0.0067795897,0.00040017554,0.00079471205,0.0076560504],"study_design_scores_gemma":[0.0000010456376,0.000016039949,0.99837434,0.0000024042865,0.0000030203914,0.000058804675,0.00025769303,0.00038561,0.00031641268,0.000058921043,0.0005237124,0.0000020283246],"about_ca_topic_score_codex":0.031975582,"about_ca_topic_score_gemma":0.06056401,"teacher_disagreement_score":0.031975582,"about_ca_system_score_codex":0.00026815003,"about_ca_system_score_gemma":0.00013413206,"threshold_uncertainty_score":0.0635789},"labels":[],"label_agreement":null},{"id":"W4415983270","doi":"10.3847/1538-4357/ae0a30","title":"Early Stellar Flybys are Unlikely: Improved Constraints from Sednoids and Large- <i>q</i> Trans-Neptunian Objects","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of British Columbia","funders":"","keywords":"Planet; Stars; Perturbation (astronomy); Ecliptic; Solar System; Orbital elements; Orbital inclination; Stellar evolution","score_opus":0.004311000760430664,"score_gpt":0.19477794971321855,"score_spread":0.19046694895278787,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415983270","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986895,0.00003963811,0.00062401,0.00004001248,0.0000027060519,0.0000028662455,0.00007284094,0.000017577886,0.0005108402],"genre_scores_gemma":[0.9993691,0.000019483505,0.00039217708,0.000011366655,0.0000028201223,0.0000022852253,0.00014660507,0.000007784959,0.00004848198],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999889,0.000025923408,0.0000075397547,0.000033983346,0.000013417271,0.000030113692],"domain_scores_gemma":[0.9991053,0.0003846774,0.00015176804,0.00010164989,0.000061833605,0.00019485097],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00046337902,0.0002970426,0.0005877785,0.0002162622,0.00060162146,0.0007666663,0.00058239856,0.00047268113,0.001032778],"category_scores_gemma":[0.0022630491,0.00021802285,0.00041829236,0.00024547736,0.0003841214,0.0008184474,0.00065648137,0.00035211688,0.00010508711],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0004991221,0.00018715518,0.5240802,0.000116029885,0.00030399294,0.0010172278,0.00041129556,0.4499971,0.011915171,0.0029604302,0.0007785693,0.0077337436],"study_design_scores_gemma":[0.00011097749,0.00015431667,0.106557846,0.00002252523,0.00010365846,0.00023429426,0.00040198176,0.88815963,0.0018714445,0.0014949592,0.0008552297,0.00003317164],"about_ca_topic_score_codex":0.00803784,"about_ca_topic_score_gemma":0.0067712264,"teacher_disagreement_score":0.00803784,"about_ca_system_score_codex":0.00035507386,"about_ca_system_score_gemma":0.0004255806,"threshold_uncertainty_score":0.015982091},"labels":[],"label_agreement":null},{"id":"W4415996851","doi":"10.3847/1538-4357/ae046d","title":"Mapping Atmospheric Features of the Planetary-mass Brown Dwarf SIMP 0136 with JWST NIRISS","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Bishop's University; Western University; Université de Montréal; McGill University","funders":"U.S. Air Force Academy; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Fonds de recherche du Québec – Nature et technologies; Canadian Space Agency; UK Research and Innovation; Space Telescope Science Institute; Mitacs; U.S. Department of Defense","keywords":"Spectral resolution; Brightness; Spectrograph; Spectral line; Spectroscopy; Principal component analysis; Spectral signature; Brown dwarf","score_opus":0.0053633261288850214,"score_gpt":0.19907857747807509,"score_spread":0.19371525134919007,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4415996851","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9986821,0.000028196073,0.00035476295,0.000011557121,0.0000014391678,0.000002107098,0.0003737215,0.00008462586,0.00046160704],"genre_scores_gemma":[0.9977093,0.000014132074,0.0010015529,0.0000046925966,0.0000035743951,0.0000020143495,0.0010902127,0.000019509907,0.00015509159],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999261,0.0000073736483,0.0000034911059,0.000025777683,0.000024749477,0.00001251899],"domain_scores_gemma":[0.9998696,0.000013912871,0.000036682002,0.000020968595,0.000023918723,0.000034805056],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015516883,0.00019739571,0.00013788295,0.0008465815,0.0002079495,0.0002364582,0.00017435636,0.0001102829,0.0006295989],"category_scores_gemma":[0.00025998012,0.00008645412,0.00022156126,0.0006099095,0.00009173214,0.00016588798,0.00027142387,0.00010205023,0.00019422184],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023916345,0.00007901499,0.87086445,0.0000384722,0.00012465635,0.00029657016,0.00041282224,0.0059480346,0.08297537,0.00032245266,0.0012613316,0.03743758],"study_design_scores_gemma":[0.000008232197,0.00002269625,0.98286414,0.0000025421514,0.000018368804,0.000064592925,0.00010730601,0.011644631,0.004030136,0.00010358643,0.001128511,0.0000051088996],"about_ca_topic_score_codex":0.009530894,"about_ca_topic_score_gemma":0.024316367,"teacher_disagreement_score":0.009530894,"about_ca_system_score_codex":0.00022394035,"about_ca_system_score_gemma":0.00017041703,"threshold_uncertainty_score":0.01895088},"labels":[],"label_agreement":null},{"id":"W4416100317","doi":"10.3847/1538-4357/adfed7","title":"The Radio Flare and Multiwavelength Afterglow of the Short GRB 231117A: Energy Injection from a Violent Shell Collision","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto; McGill University","funders":"Agence Nationale de la Recherche; European Southern Observatory; Leverhulme Trust; Canada Excellence Research Chairs, Government of Canada; National Aeronautics and Space Administration","keywords":"Afterglow; Gamma-ray burst; Flare; Blast wave; Redshift; Light curve; Shock wave; Telescope; Scintillation","score_opus":0.004356125556048183,"score_gpt":0.20588501716933794,"score_spread":0.20152889161328974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416100317","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99746764,0.000058314356,0.0014566034,0.000020727686,0.0000025005093,0.0000049871746,0.00009317657,0.000052434367,0.00084357825],"genre_scores_gemma":[0.9992187,0.000016805992,0.00042315325,0.00000492123,0.0000021897176,0.0000028028744,0.00011795272,0.000007320649,0.00020615607],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999616,0.0000034393595,0.000002354547,0.000009481209,0.000012137597,0.000010899408],"domain_scores_gemma":[0.99988115,0.000023630239,0.000044839147,0.000012740168,0.000010349478,0.00002727351],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00006765622,0.0003298205,0.00021646974,0.00044553386,0.00017415067,0.00046749623,0.0003191558,0.0002423301,0.0010159774],"category_scores_gemma":[0.00022641492,0.00015206898,0.00040762287,0.0002071909,0.00017642236,0.0001804217,0.00033695746,0.0002277417,0.00020367131],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00092546135,0.00030034358,0.6352799,0.00011172338,0.00023558013,0.0069634863,0.00033829943,0.11333153,0.1988395,0.0046023773,0.001087776,0.03798394],"study_design_scores_gemma":[0.000034802913,0.00026845947,0.702387,0.000011363343,0.00007203165,0.0014350961,0.000090372676,0.28157786,0.011645328,0.0013571354,0.001083379,0.000037259964],"about_ca_topic_score_codex":0.003989079,"about_ca_topic_score_gemma":0.0035015997,"teacher_disagreement_score":0.003989079,"about_ca_system_score_codex":0.00045558249,"about_ca_system_score_gemma":0.00011130006,"threshold_uncertainty_score":0.007931709},"labels":[],"label_agreement":null},{"id":"W4416126354","doi":"10.3847/1538-4357/ae0610","title":"Bursty or Heavy? The Surprise of Bright Population III Systems in the Reionization Era","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics","funders":"","keywords":"Reionization; Stars; Halo; Population; Star (game theory); Star formation; James Webb Space Telescope; Spitzer Space Telescope","score_opus":0.009578205099895034,"score_gpt":0.23759488700534084,"score_spread":0.2280166819054458,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416126354","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.94445175,0.0046541365,0.0037530947,0.030154737,0.0006354086,0.000011773415,0.0004977297,0.00029990572,0.015541466],"genre_scores_gemma":[0.9907312,0.0011721745,0.00081236404,0.0040449933,0.0004867674,0.000009228628,0.00018171986,0.00007883188,0.0024826438],"study_design_codex":"observational","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9999132,0.000010358666,0.0000024853925,0.00003268952,0.000017022554,0.00002423011],"domain_scores_gemma":[0.99923193,0.00015766575,0.00019049869,0.00012367585,0.00006197724,0.00023431447],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0007386203,0.00017639561,0.00022287555,0.00027846178,0.00072118646,0.0012747409,0.00036494024,0.0008969094,0.0023569693],"category_scores_gemma":[0.0020432782,0.00013618729,0.00015372531,0.00020709136,0.00088494737,0.0011004065,0.00084417005,0.0012772869,0.0009082439],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0019508388,0.0001420938,0.48027268,0.00031656076,0.00014676116,0.010611298,0.0064002187,0.0020206321,0.081173085,0.079347655,0.13730277,0.20031537],"study_design_scores_gemma":[0.00017593344,0.00047844925,0.5822595,0.0002412121,0.00012482786,0.0103711635,0.006168908,0.009516711,0.023006918,0.16487929,0.2026018,0.00017520942],"about_ca_topic_score_codex":0.0010626774,"about_ca_topic_score_gemma":0.00087045657,"teacher_disagreement_score":0.0023569693,"about_ca_system_score_codex":0.00047113575,"about_ca_system_score_gemma":0.0001326562,"threshold_uncertainty_score":0.00788486},"labels":[],"label_agreement":null},{"id":"W4416182812","doi":"10.3847/1538-4357/ae0f1d","title":"XL-Calibur Polarimetry of Cyg X-1 Further Constrains the Origin of Its Hard-state X-Ray Emission","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Swedish National Space Agency; National Aeronautics and Space Administration","keywords":"Polarimetry; Polarization (electrochemistry); Binary number; Broadband; Linear polarization; Context (archaeology)","score_opus":0.015658320650385506,"score_gpt":0.25918310331113326,"score_spread":0.24352478266074776,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416182812","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9594798,0.00038361253,0.0010919853,0.00039122,0.000017903118,0.000033523684,0.0030942548,0.00037270325,0.035134938],"genre_scores_gemma":[0.99202967,0.00007802212,0.0015355493,0.00019293817,0.000026452542,0.000013794095,0.0041340217,0.00006797557,0.0019215016],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997943,0.000019582569,0.000003773464,0.00007145479,0.000067527304,0.000043239652],"domain_scores_gemma":[0.9997099,0.00003791381,0.0000852163,0.000049237548,0.00006944971,0.000048221427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00040307618,0.00041840103,0.00021602315,0.0012389754,0.00047553756,0.0010156009,0.0002953615,0.00031514172,0.002953639],"category_scores_gemma":[0.00044397326,0.00020026555,0.0002011729,0.00062233105,0.0003973824,0.00042564777,0.0008300664,0.0005024272,0.0007113642],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001224901,0.00015378211,0.7018724,0.00013111674,0.00017519644,0.00044075746,0.0009812973,0.00449778,0.22143444,0.003892883,0.017332477,0.04786291],"study_design_scores_gemma":[0.00007554499,0.000044831882,0.9677421,0.000020672554,0.000041555588,0.00007395011,0.00012555895,0.0077347285,0.012839047,0.00025078128,0.011031941,0.000019355906],"about_ca_topic_score_codex":0.06299161,"about_ca_topic_score_gemma":0.10283651,"teacher_disagreement_score":0.06299161,"about_ca_system_score_codex":0.0018335703,"about_ca_system_score_gemma":0.00041793028,"threshold_uncertainty_score":0.12524992},"labels":[],"label_agreement":null},{"id":"W4416195862","doi":"10.3847/1538-4357/ae17b3","title":"After 54 Yr of Bar Instability Studies: A Fresh Surprise","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astronomy and Astrophysical Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"","keywords":"Instability; Halo; Bar (unit); Galaxy; Population; Range (aeronautics); Stability (learning theory)","score_opus":0.014313775238802137,"score_gpt":0.3090010231906428,"score_spread":0.2946872479518407,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416195862","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5678257,0.20873204,0.021712868,0.15336758,0.018807154,0.00013027874,0.0034749366,0.001148237,0.02480117],"genre_scores_gemma":[0.85143495,0.051083,0.009200023,0.045203995,0.015750224,0.00014182739,0.0040287958,0.0004664928,0.022690674],"study_design_codex":"design_other","study_design_gemma":"observational","domain_scores_codex":[0.99916923,0.00013995402,0.000084609994,0.00021732308,0.00020975653,0.00017917267],"domain_scores_gemma":[0.9958495,0.0008124925,0.00071611186,0.00091587426,0.0010176162,0.00068841374],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0032565733,0.0006089053,0.0011516974,0.0010106185,0.0012876696,0.001985872,0.0006970715,0.002200714,0.003757914],"category_scores_gemma":[0.006449752,0.00023378227,0.0010411235,0.0008500897,0.0013959775,0.0021977162,0.0028957522,0.0037065009,0.0032419795],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.002548409,0.0013280611,0.13178585,0.002350796,0.0014006435,0.024614973,0.006462865,0.0048578233,0.06559143,0.057987377,0.190793,0.5102789],"study_design_scores_gemma":[0.00008153764,0.0009461486,0.11131706,0.0010581557,0.00051347027,0.00916707,0.0024188,0.0024665277,0.018853828,0.05178321,0.8011804,0.00021381926],"about_ca_topic_score_codex":0.001138783,"about_ca_topic_score_gemma":0.0007572384,"teacher_disagreement_score":0.003757914,"about_ca_system_score_codex":0.0009844562,"about_ca_system_score_gemma":0.0006341291,"threshold_uncertainty_score":0.017222643},"labels":[],"label_agreement":null},{"id":"W4416233705","doi":"10.3847/1538-4357/ae0e10","title":"Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McMaster University","funders":"Natural Sciences and Engineering Research Council of Canada; National Natural Science Foundation of China; National Supercomputing Center, Korea Institute of Science and Technology Information; National Science Foundation","keywords":"Voronoi diagram; Interpolation (computer graphics); Adaptive mesh refinement; Grid; Cartesian coordinate system; Mesh generation; Star cluster; Cluster (spacecraft); Star formation","score_opus":0.02194082105039059,"score_gpt":0.26191338466146397,"score_spread":0.2399725636110734,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416233705","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.64779824,0.000096913645,0.33070403,0.00035675702,0.00021938482,0.00021227745,0.0007953355,0.0033834286,0.0164337],"genre_scores_gemma":[0.9000243,0.000039994586,0.09722195,0.00007586505,0.000016521857,0.00011660514,0.0005861466,0.00036678123,0.0015519059],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981135,0.000042451426,0.0000088561765,0.000023524532,0.00008135146,0.00003241581],"domain_scores_gemma":[0.9994942,0.00016674772,0.000045877183,0.00012804758,0.00011043435,0.000054701875],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00035775165,0.00024652836,0.0004155023,0.0002682124,0.0004819503,0.00059281813,0.0009788922,0.0003876032,0.0027142395],"category_scores_gemma":[0.0016921317,0.00018713658,0.0003839702,0.00026872792,0.00058710354,0.00033262043,0.0010367029,0.00054650434,0.0003008331],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00012964198,0.000064998996,0.0036306311,0.00004377218,0.00003236386,0.0001816029,0.00012764097,0.9671155,0.008323784,0.009200674,0.0012584466,0.009890981],"study_design_scores_gemma":[0.000026082113,0.000021556942,0.00041722308,0.000004217918,0.0000023586797,0.000016945414,0.000026028216,0.99461246,0.0023356078,0.0014147384,0.0011166304,0.000006055312],"about_ca_topic_score_codex":0.007705806,"about_ca_topic_score_gemma":0.004360262,"teacher_disagreement_score":0.007705806,"about_ca_system_score_codex":0.00050359307,"about_ca_system_score_gemma":0.000717933,"threshold_uncertainty_score":0.01532191},"labels":[],"label_agreement":null},{"id":"W4416300947","doi":"10.3847/1538-4357/ae0cb4","title":"Characterizing the Star Cluster Populations in Stephan’s Quintet Using HST and JWST Observations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University","funders":"","keywords":"Star cluster; James Webb Space Telescope; Globular cluster; Galaxy; Star formation; Photometry (optics); Spitzer Space Telescope; Cluster (spacecraft); Galaxy cluster","score_opus":0.03157353203865645,"score_gpt":0.26256981074247066,"score_spread":0.2309962787038142,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416300947","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9989729,0.000013936165,0.00013978887,0.000013425523,0.0000010730472,0.0000056092867,0.00036395664,0.000015004646,0.0004742686],"genre_scores_gemma":[0.99819905,0.0000100018415,0.000333208,0.0000076250826,0.0000019365134,0.000004076301,0.0011653728,0.000007477044,0.00027136394],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998264,0.000010819811,0.0000062997024,0.00006070756,0.00005477268,0.000040961],"domain_scores_gemma":[0.9993654,0.000057160727,0.00015301527,0.00005828956,0.00016252391,0.00020365497],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00026623916,0.00015251596,0.00013830907,0.0016833143,0.00051677914,0.00047052672,0.00044667948,0.00015070515,0.0018044079],"category_scores_gemma":[0.00079762744,0.00011011592,0.00017011732,0.0012347614,0.00024611337,0.0002986524,0.00073167594,0.00016078757,0.00037893778],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000059742775,0.000036235928,0.9844615,0.000011620399,0.00002850235,0.00036597237,0.00050139555,0.0009386009,0.005545573,0.00014661436,0.00080697803,0.007097409],"study_design_scores_gemma":[0.0000022094048,0.000013055525,0.99619424,0.000002388672,0.000003756167,0.00007003254,0.00019640962,0.0025034463,0.0004292127,0.00003941112,0.00054104463,0.000004796117],"about_ca_topic_score_codex":0.044048697,"about_ca_topic_score_gemma":0.093583085,"teacher_disagreement_score":0.044048697,"about_ca_system_score_codex":0.00049470813,"about_ca_system_score_gemma":0.00022322794,"threshold_uncertainty_score":0.087584615},"labels":[],"label_agreement":null},{"id":"W4416301680","doi":"10.3847/1538-4357/ae1008","title":"Study of H <scp>i</scp> Turbulence in the SMC Using Multipoint Structure Functions","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Université Laval","funders":"National Research Foundation of Korea","keywords":"Turbulence; Stars; Scale (ratio); Mach number; Interstellar medium; K-epsilon turbulence model; Molecular cloud","score_opus":0.01507766977000503,"score_gpt":0.2643242972480317,"score_spread":0.24924662747802667,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416301680","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9976661,0.00003303182,0.0019304841,0.000013732128,0.000002216014,0.0000028797504,0.000083727624,0.000032277414,0.0002354357],"genre_scores_gemma":[0.9995962,0.000007083192,0.00028274563,0.000002257607,0.0000033717965,8.093307e-7,0.000081527396,0.0000029225973,0.0000231321],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998946,0.00001408657,0.0000059483264,0.00003011593,0.000024569406,0.000030597308],"domain_scores_gemma":[0.99927837,0.00016614192,0.00024506132,0.00006692707,0.000106511674,0.00013700077],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00033792,0.00018187206,0.00019489284,0.0012271742,0.00026564382,0.00049099285,0.00018024957,0.00018046868,0.0004101334],"category_scores_gemma":[0.00081169925,0.00008852339,0.0003370905,0.0005758376,0.00027870908,0.00038784326,0.0003020508,0.00019107769,0.0000927317],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00013968427,0.000061857085,0.9136483,0.000025806781,0.00017034313,0.0003033589,0.00017132438,0.018909365,0.05148117,0.0014707152,0.00033735065,0.013280704],"study_design_scores_gemma":[0.0000037625946,0.000039183553,0.9036019,0.0000032823568,0.000012028677,0.000050250103,0.00007988765,0.09257421,0.0031739876,0.00029901168,0.00015000049,0.0000125150755],"about_ca_topic_score_codex":0.0045918496,"about_ca_topic_score_gemma":0.0027172007,"teacher_disagreement_score":0.0045918496,"about_ca_system_score_codex":0.0003030803,"about_ca_system_score_gemma":0.0001520484,"threshold_uncertainty_score":0.0091302395},"labels":[],"label_agreement":null},{"id":"W4416340769","doi":"10.3847/1538-4357/ae0c0c","title":"Betelgeuse, Betelgeuse, Betelgeuse, Betel-buddy? Constraints on the Dynamical Companion to <i>α</i> Orionis from HST","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Simons Foundation","keywords":"Spectrograph; Observatory; Space Telescope Imaging Spectrograph; Spectral line; Binary number; Hubble space telescope; Telescope; Stellar classification; Line (geometry); Radial velocity","score_opus":0.010692809563873206,"score_gpt":0.2323381413117507,"score_spread":0.2216453317478775,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416340769","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9984137,0.00007490576,0.00014739603,0.000017098278,0.0000027209535,0.0000016139605,0.000090582405,0.0000070198107,0.0012449933],"genre_scores_gemma":[0.9992156,0.000049536553,0.0002512279,0.000010383058,0.000007278572,0.0000011406719,0.00031841637,0.0000037899306,0.00014269867],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998783,0.000010792094,0.0000046753544,0.00004067568,0.000029951578,0.000035634144],"domain_scores_gemma":[0.9994685,0.00009626323,0.00016212965,0.00005981825,0.00004646169,0.00016679321],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00021151376,0.00012900503,0.00021126805,0.00073276553,0.00039463522,0.00079656637,0.00018139821,0.00017109908,0.0017606281],"category_scores_gemma":[0.00074834237,0.000106691026,0.000091116126,0.00043113864,0.00024257999,0.00035904575,0.0005966162,0.00022720231,0.00040995082],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003223042,0.00006808629,0.9000061,0.000043127937,0.000045118017,0.00058577996,0.0005997348,0.00047393047,0.07552501,0.0008789125,0.0004820537,0.020969769],"study_design_scores_gemma":[0.0000048559737,0.000032358388,0.99400526,0.000008991642,0.000008231616,0.00023298395,0.00023192873,0.00074314326,0.0024090311,0.00018759926,0.0021314542,0.0000041258354],"about_ca_topic_score_codex":0.0018855222,"about_ca_topic_score_gemma":0.0059192367,"teacher_disagreement_score":0.0018855222,"about_ca_system_score_codex":0.00019779343,"about_ca_system_score_gemma":0.00012704606,"threshold_uncertainty_score":0.0058898926},"labels":[],"label_agreement":null},{"id":"W4416341615","doi":"10.3847/1538-4357/ae0ffe","title":"Resolved Mass Assembly and Star Formation in Milky Way Progenitors since <i>z</i> = 5 from JWST/CANUCS: From Clumps and Mergers to Well-ordered Disks","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"Saint Mary's University; Canadian Institute for Theoretical Astrophysics; Herzberg Institute of Astrophysics; York University","funders":"","keywords":"Milky Way; Star formation; Galaxy; RADIUS; Stellar mass; Galaxy formation and evolution; Star cluster; Stellar evolution; Mass distribution","score_opus":0.007678308434641409,"score_gpt":0.23377897640094603,"score_spread":0.22610066796630462,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416341615","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9996387,0.000026744405,0.000021064638,0.0000027538772,2.1892126e-7,0.0000011820975,0.00011554094,0.0000025431336,0.0001912838],"genre_scores_gemma":[0.9994822,0.000015194471,0.00003540055,0.000002180699,6.5231706e-7,7.334597e-7,0.0003637023,0.0000016518746,0.0000983342],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989367,0.000006522245,0.0000061845553,0.000025530042,0.000029162398,0.000038920723],"domain_scores_gemma":[0.9994541,0.000040494502,0.00016275968,0.000055884702,0.00010829225,0.00017854426],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020609287,0.00013055127,0.00018402304,0.001294532,0.0004217393,0.0007758163,0.00029514782,0.00014175425,0.00078921625],"category_scores_gemma":[0.00055346004,0.000115025694,0.0001484095,0.0007963216,0.00033871617,0.00022353164,0.000713093,0.00013561748,0.0002150597],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000070995055,0.000009790523,0.99170727,0.0000040140467,0.000017281769,0.00014366434,0.00040009612,0.00011758273,0.004687245,0.00005857263,0.000055363616,0.0027281167],"study_design_scores_gemma":[9.2073213e-7,0.0000070590304,0.999212,0.0000010557171,0.0000033498,0.00006525003,0.00014498971,0.000111230875,0.00028062658,0.0000123382715,0.00015981603,0.0000013230173],"about_ca_topic_score_codex":0.051712826,"about_ca_topic_score_gemma":0.072376564,"teacher_disagreement_score":0.051712826,"about_ca_system_score_codex":0.0005988286,"about_ca_system_score_gemma":0.00028203247,"threshold_uncertainty_score":0.102823615},"labels":[],"label_agreement":null},{"id":"W4416384673","doi":"10.3847/1538-4357/ae0a37","title":"The Draco Dwarf Spheroidal Galaxy in the First Year of Dark Energy Spectroscopic Instrument Data","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"High Energy Physics; Natural Sciences and Engineering Research Council of Canada; National Science and Technology Council; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; U.S. Department of Energy; Ministerio de Ciencia, Innovación y Universidades; Gordon and Betty Moore Foundation; Agencia Estatal de Investigación; Office of Science; Science and Technology Facilities Council; Division of Astronomical Sciences; Ministry of Education, India; National Science Foundation","keywords":"Metallicity; Dwarf spheroidal galaxy; Surface brightness; Velocity dispersion; Galaxy; Stars; RADIUS; Dwarf galaxy; Red-giant branch","score_opus":0.008133254405110688,"score_gpt":0.22355863144238705,"score_spread":0.21542537703727638,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416384673","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99871993,0.000041873376,0.000047050686,0.0000344578,0.0000017718613,0.0000018297127,0.0005518956,0.0000088258785,0.0005922785],"genre_scores_gemma":[0.9981906,0.000020647678,0.0000681834,0.000012822268,0.0000018593811,0.0000013335205,0.001404166,0.0000037518037,0.00029659603],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997497,0.000039373805,0.000013730316,0.00006514652,0.000062292434,0.00006971879],"domain_scores_gemma":[0.9986608,0.00013970096,0.00044339962,0.00014822242,0.00027515928,0.0003327453],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00049477746,0.00012519585,0.00020996196,0.00084730977,0.00032269175,0.0005907867,0.0001815311,0.0001477456,0.0007084622],"category_scores_gemma":[0.0012809956,0.00010664007,0.00013950578,0.00075058395,0.00022519573,0.00021373322,0.0005218009,0.00014661501,0.00031875412],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00003457988,0.0000055595015,0.996763,0.000004191636,0.000010555414,0.00007828726,0.00013143712,0.000094068615,0.0010713052,0.00003995404,0.00021763952,0.0015493813],"study_design_scores_gemma":[7.197083e-7,0.0000111169265,0.9989391,0.0000018018715,0.0000028469688,0.000048265418,0.00010832351,0.00023242555,0.00014234729,0.000009833762,0.0005018214,0.000001450563],"about_ca_topic_score_codex":0.04518314,"about_ca_topic_score_gemma":0.08806164,"teacher_disagreement_score":0.04518314,"about_ca_system_score_codex":0.00056238956,"about_ca_system_score_gemma":0.00023442354,"threshold_uncertainty_score":0.08984029},"labels":[],"label_agreement":null},{"id":"W4416396869","doi":"10.3847/1538-4357/ae0a22","title":"On the Fe <scp>xxii</scp> Emission in the X-Ray Spectrum of NGC 1068","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Active galactic nucleus; Galaxy; Context (archaeology); Photoionization; Emission spectrum; Line (geometry); Ionization; Spectral line","score_opus":0.010535074127428408,"score_gpt":0.23541424290105062,"score_spread":0.2248791687736222,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416396869","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.997948,0.000029166227,0.00016665815,0.000038871007,0.0000021232918,0.0000014358418,0.0002764081,0.00005130273,0.0014861488],"genre_scores_gemma":[0.9994522,0.000009909297,0.00019001552,0.000008809032,0.0000017431648,7.2366606e-7,0.00018930342,0.000006031848,0.00014117954],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999496,0.0000071176437,0.0000033006024,0.000016826709,0.00001389685,0.0000092452465],"domain_scores_gemma":[0.99977165,0.000057338722,0.0000814542,0.000029854933,0.00002046414,0.000039247276],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00011439531,0.00016578156,0.00011018882,0.00039337002,0.00015926658,0.00029472186,0.00017614033,0.00018692348,0.0015198193],"category_scores_gemma":[0.00029006487,0.00008283684,0.00010970204,0.0002895319,0.00016787718,0.00015576788,0.00020227404,0.00015362684,0.00034995633],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0003648936,0.00009864739,0.78923124,0.00006429082,0.000069548376,0.0012089967,0.00029328666,0.0061071883,0.18666884,0.000912643,0.001379143,0.013601286],"study_design_scores_gemma":[0.00000518129,0.00003484432,0.993763,0.0000055809696,0.0000070240644,0.00022277018,0.000042842494,0.0030824293,0.0021730186,0.00012383146,0.000535628,0.0000038401035],"about_ca_topic_score_codex":0.0021580604,"about_ca_topic_score_gemma":0.0031419143,"teacher_disagreement_score":0.0021580604,"about_ca_system_score_codex":0.00019201133,"about_ca_system_score_gemma":0.000036831727,"threshold_uncertainty_score":0.005084336},"labels":[],"label_agreement":null},{"id":"W4416565618","doi":"10.3847/1538-4357/ae0ca3","title":"Spectrotemporal Analysis of X-Ray Reverberation in the Seyfert 1.5 Galaxy 4U 1344–60","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Saint Mary's University","funders":"","keywords":"Reverberation mapping; Galaxy; Reverberation; Flux (metallurgy); Accretion (finance); Spectral line; Black hole (networking); Accretion disc","score_opus":0.010496481863576726,"score_gpt":0.2523088075929845,"score_spread":0.2418123257294078,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416565618","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9958882,0.000121431236,0.0021743649,0.00007548765,0.000011943141,0.000006631011,0.0004030924,0.00032278066,0.0009960366],"genre_scores_gemma":[0.99775213,0.000043262546,0.000983854,0.000020772884,0.000010265725,0.000005840371,0.00080598664,0.00006865478,0.00030919307],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99991345,0.000010708854,0.0000037281645,0.000029102936,0.000022058824,0.000020986841],"domain_scores_gemma":[0.99980766,0.000032359596,0.0000605364,0.000032124157,0.00003120313,0.000036079775],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00036997016,0.00041057743,0.00024606715,0.0012989326,0.0002262915,0.00037638843,0.00029033076,0.00029690214,0.0015078131],"category_scores_gemma":[0.00060453854,0.00020843883,0.00062191003,0.00046972945,0.0001866122,0.00022998336,0.0002828241,0.00025053933,0.000349335],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006436768,0.00019018777,0.7799562,0.00016486384,0.0005314946,0.0008654306,0.0007675326,0.04319847,0.12854207,0.0022205291,0.003225531,0.039693937],"study_design_scores_gemma":[0.000015428073,0.000103860744,0.95081306,0.000011594788,0.00006339326,0.0001390322,0.0001050238,0.043343082,0.0035584099,0.00031152295,0.0015117365,0.000023780456],"about_ca_topic_score_codex":0.007205799,"about_ca_topic_score_gemma":0.008240742,"teacher_disagreement_score":0.007205799,"about_ca_system_score_codex":0.00052492844,"about_ca_system_score_gemma":0.00015949574,"threshold_uncertainty_score":0.014327705},"labels":[],"label_agreement":null},{"id":"W4416565648","doi":"10.3847/1538-4357/ae0e54","title":"Gravitational Redshift for Rapidly Rotating Neutron Stars","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Alberta","funders":"","keywords":"Neutron star; Pulsar; Schwarzschild radius; Redshift; RADIUS; Gravitational redshift; Schwarzschild metric; Flux (metallurgy)","score_opus":0.012344348990618976,"score_gpt":0.32763170044082934,"score_spread":0.31528735145021036,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416565648","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.97051954,0.0008648165,0.016847745,0.00021994607,0.00004584461,0.0000115832,0.00038841847,0.00013985852,0.010962384],"genre_scores_gemma":[0.99451786,0.00023212159,0.003903582,0.000033802247,0.000022958438,0.0000073270003,0.00049103785,0.000028113816,0.00076313823],"study_design_codex":"observational","study_design_gemma":"theoretical_or_conceptual","domain_scores_codex":[0.9996667,0.0000941697,0.000020158173,0.00007796808,0.0001009622,0.000040063132],"domain_scores_gemma":[0.99866617,0.00044858977,0.00052072376,0.00014512487,0.00013682884,0.000082575156],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0012020511,0.00024088827,0.00027212035,0.0015152971,0.00037123536,0.00047952434,0.0002965935,0.00027536784,0.001126635],"category_scores_gemma":[0.004206123,0.0001288559,0.00034403635,0.00065088755,0.00037730936,0.0003824233,0.0008390457,0.00032808873,0.00030747268],"study_design_candidate":"theoretical_or_conceptual","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00033050758,0.000041223928,0.6159748,0.00017154016,0.0001293388,0.0007049013,0.00066567975,0.11281083,0.034688007,0.17422916,0.0022776148,0.057976387],"study_design_scores_gemma":[0.00006531356,0.00023128542,0.6686907,0.0000932962,0.00005523691,0.0009463337,0.00024056829,0.23120551,0.013221311,0.064358145,0.020806242,0.000086167456],"about_ca_topic_score_codex":0.005887071,"about_ca_topic_score_gemma":0.0034857471,"teacher_disagreement_score":0.005887071,"about_ca_system_score_codex":0.000852176,"about_ca_system_score_gemma":0.00022833789,"threshold_uncertainty_score":0.011705577},"labels":[],"label_agreement":null},{"id":"W4416616962","doi":"10.3847/1538-4357/ae07cd","title":"So Long Kolmogorov: The Forward and Backward Turbulence Cascades in a Supernovae-driven, Multiphase Interstellar Medium","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":4,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Cascade; Interstellar medium; Supernova; Turbulence; Flux (metallurgy); Energy cascade; Galaxy; Inverse","score_opus":0.00816813489044585,"score_gpt":0.25130190015062914,"score_spread":0.2431337652601833,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416616962","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98975974,0.00008962521,0.0051482576,0.00021616233,0.000054325246,0.000027636603,0.000083291605,0.0000927149,0.0045283413],"genre_scores_gemma":[0.9986369,0.000030038518,0.0007803319,0.000029676472,0.000007414683,0.000009851867,0.00003603072,0.0000128428865,0.00045696858],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99992704,0.000015890457,0.0000032448927,0.000011406173,0.000015759384,0.000026689379],"domain_scores_gemma":[0.9997775,0.00006089449,0.000041448686,0.000015535017,0.000027228767,0.00007745222],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001757206,0.000344268,0.0003305464,0.00032055276,0.00058021833,0.0010509363,0.0004628111,0.0005679016,0.0015611545],"category_scores_gemma":[0.0007394655,0.00023017927,0.0005435536,0.00014765644,0.000770146,0.0007277844,0.0008139787,0.0005994941,0.00009921193],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00023956993,0.00014999196,0.009990196,0.000035059435,0.00009627265,0.0004917717,0.00013628742,0.96013737,0.0150735425,0.011302953,0.0005934861,0.001753491],"study_design_scores_gemma":[0.000043267424,0.00004014441,0.0022396562,0.00000315778,0.00000863245,0.0000171129,0.00003499755,0.9952435,0.0009186163,0.0012659194,0.0001746948,0.000010282658],"about_ca_topic_score_codex":0.008242044,"about_ca_topic_score_gemma":0.0041249343,"teacher_disagreement_score":0.008242044,"about_ca_system_score_codex":0.0005465952,"about_ca_system_score_gemma":0.00064318365,"threshold_uncertainty_score":0.016388118},"labels":[],"label_agreement":null},{"id":"W4416729173","doi":"10.3847/1538-4357/ae0615","title":"The JWST Early Release Science Program for Direct Observations of Exoplanetary Systems. VI. Evidence for Radially Evolving Icy Grains in the HD 141569A Disk via NIRCam Coronagraphic Imaging","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Western University; Herzberg Institute of Astrophysics","funders":"Space Telescope Science Institute; National Aeronautics and Space Administration","keywords":"Exoplanet; Planet; Circumstellar disk; Planetary system; James Webb Space Telescope; Deconvolution; Stars","score_opus":0.025786569824020677,"score_gpt":0.2950825104372995,"score_spread":0.26929594061327883,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416729173","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.690384,0.002101203,0.018033054,0.0037453778,0.00052998704,0.002126468,0.17618835,0.0069250516,0.09996658],"genre_scores_gemma":[0.631043,0.00094684015,0.08331887,0.0014593718,0.00055367185,0.0011561477,0.23064105,0.0016742339,0.049206853],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.99963164,0.000026398577,0.000020639363,0.000052716372,0.00020640023,0.00006215566],"domain_scores_gemma":[0.9985195,0.00010262677,0.00024621043,0.0003221038,0.0002945281,0.0005151879],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0013598987,0.00047436522,0.0003692311,0.0017319757,0.0006543747,0.0006620169,0.0007576051,0.00037409188,0.013948186],"category_scores_gemma":[0.0008406238,0.00031108587,0.00036594097,0.0011283101,0.00021974459,0.00067979365,0.0014900195,0.0006723942,0.0044847704],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011784193,0.0009884282,0.2647073,0.0005296854,0.0003009064,0.002039835,0.00080840936,0.0012900702,0.3700364,0.0021653548,0.18741271,0.1685425],"study_design_scores_gemma":[0.0002958525,0.00025383846,0.8786399,0.000053262618,0.000051993477,0.0005314957,0.00013994447,0.002529686,0.012921277,0.00079474715,0.10375648,0.000031470743],"about_ca_topic_score_codex":0.006568125,"about_ca_topic_score_gemma":0.03514285,"teacher_disagreement_score":0.013948186,"about_ca_system_score_codex":0.0006067979,"about_ca_system_score_gemma":0.00066626247,"threshold_uncertainty_score":0.046661258},"labels":[],"label_agreement":null},{"id":"W4416771371","doi":"10.3847/1538-4357/ae12f3","title":"First X-Ray and Radio Polarimetry of the Neutron Star Low-mass X-Ray Binary GX 17+2","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Lethbridge; McGill University","funders":"National Aeronautics and Space Administration","keywords":"Polarimetry; Neutron star; Polarization (electrochemistry); Binary number; Accretion disc; Accretion (finance); Telescope; Binary star","score_opus":0.006326431802237579,"score_gpt":0.21335468897220455,"score_spread":0.20702825716996698,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416771371","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99543947,0.00038961315,0.00073411624,0.000031725252,0.000009266978,0.000012257355,0.00027378538,0.000024068275,0.003085607],"genre_scores_gemma":[0.9967796,0.00016524401,0.0012736389,0.00003584264,0.000020017507,0.000009208259,0.00088924373,0.00002031729,0.00080693257],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9999032,0.00001686577,0.000005167468,0.000022075666,0.00003205558,0.00002064554],"domain_scores_gemma":[0.99977607,0.00003177334,0.0000780837,0.000028803952,0.000047278474,0.00003794019],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00028476652,0.000274941,0.00024916005,0.0008780596,0.00044795102,0.0006733939,0.00015446483,0.00022480058,0.0010245802],"category_scores_gemma":[0.00031721772,0.00020031234,0.00014945798,0.00047197385,0.00033585995,0.00025851367,0.0007078639,0.00032525096,0.00035997335],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001437602,0.00010149715,0.47079566,0.00018488032,0.00015588586,0.0018594923,0.0006147975,0.00082575245,0.49768418,0.0012678453,0.0006658666,0.024406672],"study_design_scores_gemma":[0.00005447076,0.0003617701,0.94981045,0.000036526682,0.00007774069,0.0014120955,0.0002614893,0.00091395905,0.04073226,0.00030567904,0.0060181012,0.000015473584],"about_ca_topic_score_codex":0.0007232477,"about_ca_topic_score_gemma":0.0012946627,"teacher_disagreement_score":0.0010245802,"about_ca_system_score_codex":0.00020340504,"about_ca_system_score_gemma":0.00014001525,"threshold_uncertainty_score":0.003427565},"labels":[],"label_agreement":null},{"id":"W4416771401","doi":"10.3847/1538-4357/ae1003","title":"WALLABY Pilot Survey: Characterizing Low-rotation Kinematically Modeled Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba; Western University; University of Toronto; Arthur B. McDonald-Canadian Astroparticle Physics Research Institute; Queen's University","funders":"","keywords":"Kinematics; Galaxy; Rotation (mathematics); Scaling; Universe; Galaxy rotation curve; Galaxy formation and evolution","score_opus":0.011800471996927867,"score_gpt":0.23044517132546996,"score_spread":0.21864469932854208,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416771401","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9902154,0.00009767953,0.0031658718,0.00014016093,0.00000749908,0.000045775538,0.0036914248,0.0005481178,0.0020879142],"genre_scores_gemma":[0.98347753,0.000058859107,0.004787725,0.00010266367,0.000018987046,0.00006875633,0.010663971,0.00020788271,0.0006135937],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99918824,0.0002236734,0.000034151635,0.00020644173,0.00017570464,0.00017178524],"domain_scores_gemma":[0.9970913,0.00044209926,0.00082456256,0.0008989564,0.00030856775,0.00043447188],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0017457829,0.0004409916,0.0003470527,0.001293017,0.00064491096,0.00093828625,0.0008659364,0.00030270978,0.0013409173],"category_scores_gemma":[0.0043689087,0.000293574,0.00026006193,0.0010663692,0.00062207517,0.0007021617,0.0015710936,0.00040732414,0.0012185698],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00030017892,0.0000921705,0.95969594,0.00004172982,0.000058777696,0.00021635948,0.0010792712,0.0057935542,0.0036104992,0.0017130786,0.0089602135,0.01843828],"study_design_scores_gemma":[0.00008657607,0.00014232766,0.9518793,0.00005221312,0.000031231622,0.00019108276,0.000695316,0.034744475,0.0023459005,0.0011358551,0.008657,0.000038715298],"about_ca_topic_score_codex":0.030022757,"about_ca_topic_score_gemma":0.023887295,"teacher_disagreement_score":0.030022757,"about_ca_system_score_codex":0.0006214375,"about_ca_system_score_gemma":0.0005539551,"threshold_uncertainty_score":0.05969602},"labels":[],"label_agreement":null},{"id":"W4416771448","doi":"10.3847/1538-4357/ae0619","title":"ALMA-IMF. XX. Core Fragmentation in the W51 High-mass Star-forming Region","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Fragmentation (computing); Equipartition theorem; Thermal; Core (optical fiber); H II region; Flux (metallurgy)","score_opus":0.014843249483677943,"score_gpt":0.26419517907416357,"score_spread":0.24935192959048563,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416771448","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9890042,0.00012451588,0.00080373907,0.000046550376,0.000008068209,0.000011756025,0.0022547054,0.00011056689,0.0076360055],"genre_scores_gemma":[0.99488527,0.000035664358,0.0006992868,0.000013985716,0.0000046995465,0.000007734496,0.0022513596,0.00003120842,0.0020706926],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99993145,0.000011844996,0.0000050216036,0.000014847734,0.000013508125,0.00002337688],"domain_scores_gemma":[0.9997162,0.000046159723,0.00009309975,0.000041752253,0.000067677334,0.000035104313],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00027449237,0.00010726331,0.00009492476,0.0006410974,0.0002345919,0.00044519527,0.00015932019,0.0001388809,0.0038094274],"category_scores_gemma":[0.00083386805,0.000051018644,0.0001489248,0.00045703963,0.00007649019,0.00021132607,0.00021588951,0.0001045378,0.0011501516],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00045872753,0.00004277179,0.93781406,0.000046714944,0.00010699614,0.00031648655,0.00018066529,0.003489291,0.009309601,0.001478141,0.0040117335,0.04274486],"study_design_scores_gemma":[0.000008600446,0.000032193147,0.9837933,0.000010754424,0.000015336735,0.00016960318,0.00011384633,0.009603156,0.0016128452,0.00022396121,0.0044126725,0.0000036490385],"about_ca_topic_score_codex":0.006835742,"about_ca_topic_score_gemma":0.0066203335,"teacher_disagreement_score":0.006835742,"about_ca_system_score_codex":0.00028614062,"about_ca_system_score_gemma":0.00013076469,"threshold_uncertainty_score":0.013591886},"labels":[],"label_agreement":null},{"id":"W4416774226","doi":"10.3847/1538-4357/ae0d83","title":"Galaxy Model Subtraction with a Convolutional Denoising Autoencoder","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Generative Adversarial Networks and Image Synthesis","field":"Computer Science","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Herzberg Institute of Astrophysics","funders":"","keywords":"Galaxy; Convolutional neural network; Residual; Pattern recognition (psychology); Spiral galaxy; Ellipse; Subtraction; Background subtraction","score_opus":0.009253971442445804,"score_gpt":0.2236433382282354,"score_spread":0.2143893667857896,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416774226","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.07069694,0.00025344896,0.9223559,0.00035991354,0.0001049747,0.000048756727,0.0002500532,0.003573104,0.0023570133],"genre_scores_gemma":[0.7205208,0.00014603371,0.2709852,0.00043847837,0.000061472376,0.000079708894,0.0012424757,0.00030667,0.006219071],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99981076,0.000026279935,0.000007655304,0.00006682002,0.000052756,0.000035780133],"domain_scores_gemma":[0.99962676,0.00013387839,0.000033717468,0.0000765663,0.00010390547,0.000025177878],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00061062136,0.0008647932,0.0005489712,0.0003944515,0.00019384407,0.000460071,0.0011622637,0.0008828191,0.001555693],"category_scores_gemma":[0.001454038,0.00038416023,0.00070246786,0.00031385035,0.0004452944,0.0005055199,0.00084124284,0.0013334132,0.00081225747],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00011737322,0.0000544926,0.0012181931,0.000037827507,0.000085855136,0.000061369785,0.000038303093,0.86937886,0.012130469,0.0032658463,0.001854571,0.11175683],"study_design_scores_gemma":[0.000002037615,0.000007818071,0.00010464435,0.0000018422753,0.000003166115,0.000007156601,0.0000014670288,0.99735296,0.0018284479,0.00049127225,0.00019696633,0.0000022459812],"about_ca_topic_score_codex":0.008535909,"about_ca_topic_score_gemma":0.00799652,"teacher_disagreement_score":0.008535909,"about_ca_system_score_codex":0.0007630316,"about_ca_system_score_gemma":0.000600735,"threshold_uncertainty_score":0.016972482},"labels":[],"label_agreement":null},{"id":"W4416797708","doi":"10.3847/1538-4357/ae100a","title":"The ZZ Ceti Instability Strip for the Most Massive White Dwarf Pulsators","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"Science and Technology Facilities Council; Instituto de Astrofísica de Canarias; Vlaamse regering; Fonds Wetenschappelijk Onderzoek; Consejo Nacional de Investigaciones Científicas y Técnicas; Agència de Gestió d'Ajuts Universitaris i de Recerca; Agencia Nacional de Promoción de la Investigación, el Desarrollo Tecnológico y la Innovación; National Science Foundation; Generalitat de Catalunya; National Aeronautics and Space Administration","keywords":"Instability strip; White dwarf; Photometry (optics); Instability; Stars; Amplitude; Asteroseismology","score_opus":0.009663114268230747,"score_gpt":0.2403951460013174,"score_spread":0.23073203173308665,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416797708","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9967591,0.00012441011,0.00022981176,0.000020253283,0.000001948446,0.000006930335,0.001548862,0.000035731493,0.001272949],"genre_scores_gemma":[0.99789834,0.00003747418,0.00016259422,0.0000039460147,0.000003346289,0.000004122287,0.0015463319,0.0000052801292,0.00033853648],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998822,0.0000054169786,0.0000066052467,0.000038157814,0.000037712973,0.000029997489],"domain_scores_gemma":[0.9992937,0.000058780737,0.00035179374,0.00005502337,0.00010124169,0.00013949464],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00015311528,0.00017707035,0.00017596154,0.0017767011,0.00033119653,0.00056727027,0.00022933609,0.00012064331,0.0020317151],"category_scores_gemma":[0.0008080008,0.00009912815,0.00014595091,0.0011288926,0.00017371203,0.0001594845,0.0003975002,0.00012221654,0.00035812875],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00009781589,0.00000938844,0.98306227,0.0000149580255,0.000018959889,0.000105216706,0.00015445794,0.0001846382,0.007415767,0.000079173544,0.00046320615,0.008394138],"study_design_scores_gemma":[7.0775667e-7,0.00000498939,0.9991953,0.0000010709517,0.0000031428071,0.00003913587,0.000030076877,0.00020164132,0.00027390206,0.000011117233,0.0002377638,0.0000011556891],"about_ca_topic_score_codex":0.03237964,"about_ca_topic_score_gemma":0.054495562,"teacher_disagreement_score":0.03237964,"about_ca_system_score_codex":0.00055822823,"about_ca_system_score_gemma":0.00023022294,"threshold_uncertainty_score":0.064382315},"labels":[],"label_agreement":null},{"id":"W4416914199","doi":"10.3847/1538-4357/ae145f","title":"Discovery of a Little Red Dot Candidate at <i>z</i>  ≳ 10 in COSMOS-web Based on MIRI-NIRCam Selection","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysical Phenomena and Observations","field":"Physics and Astronomy","cited_by":6,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Japan Society for the Promotion of Science; Agencia Nacional de Investigación y Desarrollo; Ministry of Education, Culture, Sports, Science and Technology; Centre National d’Etudes Spatiales; European Commission; National Natural Science Foundation of China; National Research Foundation; Astronomical Society of Japan; Danmarks Grundforskningsfond; National Aeronautics and Space Administration; Deutsche Forschungsgemeinschaft; Space Telescope Science Institute; National Science Foundation","keywords":"Photometry (optics); James Webb Space Telescope; Population; Supermassive black hole; Selection (genetic algorithm); Predictability","score_opus":0.006974562934420476,"score_gpt":0.22832838821137727,"score_spread":0.2213538252769568,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416914199","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99041253,0.00034371746,0.0024417224,0.00016114875,0.000048777914,0.00003681441,0.000916579,0.00044910808,0.0051896046],"genre_scores_gemma":[0.9946661,0.00004324859,0.0022773775,0.00012656719,0.000029197145,0.000015356187,0.0017060634,0.00006752432,0.0010685674],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971074,0.000015881293,0.000012682867,0.000098372635,0.0000762651,0.00008606503],"domain_scores_gemma":[0.99919087,0.00007081728,0.00018329741,0.0000900921,0.00010045259,0.00036455356],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00048388873,0.00034703137,0.0005102971,0.001996365,0.0008569048,0.0012156587,0.00047707083,0.0004479002,0.0029788862],"category_scores_gemma":[0.0004791259,0.00025830866,0.0005100323,0.0010776904,0.00032857925,0.00030194482,0.0010027369,0.00030928783,0.0014832675],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0006689377,0.0002157765,0.85839146,0.00014524092,0.00018090736,0.005834473,0.00058564596,0.00046076236,0.09394007,0.001580677,0.008812707,0.029183412],"study_design_scores_gemma":[0.000067347275,0.00013036127,0.9600019,0.000031259802,0.00015787425,0.0030312364,0.0004385722,0.0054113595,0.017243378,0.00041723685,0.013027348,0.000042189244],"about_ca_topic_score_codex":0.0020845274,"about_ca_topic_score_gemma":0.0043782503,"teacher_disagreement_score":0.0029788862,"about_ca_system_score_codex":0.00028204886,"about_ca_system_score_gemma":0.00016878243,"threshold_uncertainty_score":0.00996536},"labels":[],"label_agreement":null},{"id":"W4416958515","doi":"10.3847/1538-4357/ae0d87","title":"Gaussian Process Methods for Very Large Astrometric Data Sets","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gaussian Processes and Bayesian Inference","field":"Computer Science","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Queen's University","funders":"","keywords":"Velocity dispersion; Gaussian process; Gaussian; Dispersion (optics); Radial velocity; Stars; Milky Way; Tensor (intrinsic definition)","score_opus":0.03078282036648877,"score_gpt":0.3748417231400589,"score_spread":0.34405890277357015,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416958515","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.006292736,0.00015942767,0.99249345,0.0001731327,0.000019993151,0.00004906708,0.00019325716,0.00046395365,0.00015504056],"genre_scores_gemma":[0.2656235,0.00045622783,0.72682065,0.0003269579,0.00026929355,0.0008737611,0.0029393744,0.00038493235,0.0023052986],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99468637,0.0026755664,0.00028722722,0.0010897359,0.0009585474,0.0003025706],"domain_scores_gemma":[0.97570384,0.01845388,0.0014393977,0.002514557,0.0015091924,0.00037915446],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.015990619,0.001362838,0.0024615605,0.0034586806,0.0012356302,0.002294878,0.004993778,0.002652391,0.002511325],"category_scores_gemma":[0.03381308,0.0018840205,0.00300433,0.0034200249,0.0027974916,0.0027648362,0.0042402563,0.004401398,0.001021743],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001227752,0.000101091,0.0039033622,0.00013950291,0.00025487551,0.00016889337,0.00015734129,0.87816834,0.0010071008,0.04384735,0.0020587046,0.07007067],"study_design_scores_gemma":[0.000006732674,0.000008901974,0.00017867191,0.000005874594,0.0000037979398,0.0000072456655,0.000008524837,0.9855155,0.00010588656,0.013864084,0.00028820444,0.000006711109],"about_ca_topic_score_codex":0.016934333,"about_ca_topic_score_gemma":0.014819119,"teacher_disagreement_score":0.016934333,"about_ca_system_score_codex":0.0019478644,"about_ca_system_score_gemma":0.002579699,"threshold_uncertainty_score":0.08456749},"labels":[],"label_agreement":null},{"id":"W4416976360","doi":"10.3847/1538-4357/ae160d","title":"The Photometric Analysis of the Environment Around Two Dusty Star-forming Galaxies at <i>z</i>  ∼ 2","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Waterloo; University of British Columbia","funders":"European Regional Development Fund; Natural Sciences and Engineering Research Council of Canada; Narodowa Agencja Wymiany Akademickiej; National Science Foundation; Korea Astronomy and Space Science Institute; Ministério da Ciência, Tecnologia, Inovações e Comunicações; Agencia Estatal de Investigación; Agencia Nacional de Investigación y Desarrollo; Ministerio de Ciencia, Innovación y Universidades","keywords":"Galaxy; Hubble space telescope; Stellar mass; Photometry (optics); Star formation; TRACE (psycholinguistics); Galaxy formation and evolution","score_opus":0.0058680973672653155,"score_gpt":0.21271632557140832,"score_spread":0.206848228204143,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416976360","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99907625,0.000016417944,0.00010259366,0.000006073249,7.173429e-7,0.0000018276723,0.00018198042,0.000014323931,0.0005999504],"genre_scores_gemma":[0.99912995,0.000009991588,0.0002993491,0.000007008773,0.000002016435,0.0000013079477,0.00044358446,0.0000034475809,0.00010329781],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999199,0.000005259298,0.000003534231,0.000025222565,0.000020264215,0.00002582309],"domain_scores_gemma":[0.9997297,0.000025539006,0.0000887569,0.000025946607,0.00003301046,0.00009697494],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00012129574,0.00012387936,0.00012608143,0.0009407449,0.0002955632,0.00040712056,0.00018521196,0.00012723579,0.0009433568],"category_scores_gemma":[0.0002358658,0.00010704985,0.000111985326,0.00048463492,0.00021163115,0.00015662098,0.00039117548,0.00013568682,0.00019604951],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0001312832,0.000029962159,0.9462265,0.0000150266005,0.000029776429,0.00019950584,0.00026970007,0.00025300193,0.045467697,0.00014617486,0.00031155223,0.006919885],"study_design_scores_gemma":[0.00000202065,0.000010668961,0.9981933,9.875192e-7,0.000005678057,0.000059072834,0.000065988366,0.00022564737,0.0011932631,0.000012143445,0.00022997874,0.0000010462579],"about_ca_topic_score_codex":0.007522394,"about_ca_topic_score_gemma":0.011289409,"teacher_disagreement_score":0.007522394,"about_ca_system_score_codex":0.00031118406,"about_ca_system_score_gemma":0.0001085848,"threshold_uncertainty_score":0.014957249},"labels":[],"label_agreement":null},{"id":"W4416977891","doi":"10.3847/1538-4357/ae1020","title":"Detection of CH <mml:math xmlns:mml=\"http://www.w3.org/1998/Math/MathML\"> <mml:msubsup> <mml:mrow/> <mml:mrow> <mml:mn>3</mml:mn> </mml:mrow> <mml:mrow> <mml:mo>+</mml:mo> </mml:mrow> </mml:msubsup> </mml:math> in the O-rich Planetary Nebula NGC 6302","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Naval Research; Agencia Estatal de Investigación; Science and Technology Facilities Council; Natural Sciences and Engineering Research Council of Canada; Irish Research Council; Ministerio de Ciencia, Innovación y Universidades; California Institute of Technology; National Aeronautics and Space Administration; Science Foundation Ireland; UK Research and Innovation; Canadian Space Agency; Jet Propulsion Laboratory; Space Telescope Science Institute; National Science Foundation","keywords":"Planetary nebula; Nebula; Astrochemistry; Planetary system; Emission nebula; Excitation; Stars; Spectrometer","score_opus":0.012198709462347204,"score_gpt":0.23019611296201306,"score_spread":0.21799740349966584,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4416977891","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9734423,0.00088595017,0.004158438,0.00047677223,0.00010318886,0.0000600383,0.004923743,0.0007619616,0.0151876835],"genre_scores_gemma":[0.9835616,0.00021370324,0.006134823,0.0005561048,0.000026318692,0.000036558224,0.0024507775,0.00011638073,0.0069037657],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9997899,0.000012792426,0.000010859318,0.00007681812,0.00006506624,0.000044607732],"domain_scores_gemma":[0.99973077,0.000049980783,0.000051029354,0.00005596141,0.00005109787,0.00006111382],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00022782249,0.00024167365,0.00014632884,0.00066851755,0.00046825063,0.00048551784,0.00034059232,0.0010655634,0.0074203713],"category_scores_gemma":[0.00043136705,0.00019306272,0.00017778785,0.00032484625,0.00024878618,0.00023612523,0.00062065886,0.00036284162,0.0016741842],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00038676494,0.000064640575,0.18574715,0.000115219125,0.0000706926,0.0011932653,0.00033737745,0.000326816,0.78826463,0.0004988636,0.0066440785,0.016350543],"study_design_scores_gemma":[0.00006633988,0.00034750666,0.58651716,0.00008199557,0.0000898423,0.0026815445,0.0005246621,0.003140873,0.3510272,0.00087707513,0.054584306,0.000061526334],"about_ca_topic_score_codex":0.0059066718,"about_ca_topic_score_gemma":0.0137867965,"teacher_disagreement_score":0.0074203713,"about_ca_system_score_codex":0.0003031699,"about_ca_system_score_gemma":0.00018995526,"threshold_uncertainty_score":0.024823606},"labels":[],"label_agreement":null},{"id":"W4417102054","doi":"10.3847/1538-4357/ae1602","title":"The Role of the Secondary White Dwarf in a Double-degenerate Double-detonation Explosion, in the Supernova Remnant Phase","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Manitoba","funders":"","keywords":"Ejecta; White dwarf; Supernova; Supernova remnant; Primary (astronomy); Detonation; Spectroscopy; Phase (matter)","score_opus":0.011167291375280757,"score_gpt":0.25338765947007275,"score_spread":0.242220368094792,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417102054","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99725014,0.00007132184,0.0009897436,0.00002924378,0.000007772292,0.000005313796,0.000062073435,0.00003991814,0.001544467],"genre_scores_gemma":[0.99935645,0.000021315542,0.00019175447,0.000005327224,0.0000018285685,0.0000018469868,0.000056437573,0.000008166006,0.00035693735],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.999964,0.0000056642243,0.0000019633105,0.000009439441,0.000007378571,0.000011644378],"domain_scores_gemma":[0.99985516,0.000022270473,0.000028871304,0.000013503475,0.00001704109,0.00006313552],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001548766,0.0002880429,0.00026425876,0.00020121278,0.0003189359,0.00091514195,0.00023602978,0.00038674986,0.0016538296],"category_scores_gemma":[0.0005035558,0.00016864053,0.00031220657,0.00011337829,0.0003322151,0.00038705824,0.000592057,0.0002525886,0.00022558469],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.001921646,0.0005958423,0.27096388,0.00022654164,0.00040923472,0.0077949157,0.0005753527,0.4986073,0.1813262,0.019938432,0.0015861057,0.016054599],"study_design_scores_gemma":[0.00020779815,0.00085664314,0.2289356,0.000040829316,0.00018892398,0.0012543214,0.00054635276,0.7362404,0.022612233,0.005712264,0.0033359835,0.00006866585],"about_ca_topic_score_codex":0.0029102932,"about_ca_topic_score_gemma":0.001495847,"teacher_disagreement_score":0.0029102932,"about_ca_system_score_codex":0.0002748223,"about_ca_system_score_gemma":0.00022293504,"threshold_uncertainty_score":0.0057867765},"labels":[],"label_agreement":null},{"id":"W4417147191","doi":"10.3847/1538-4357/ae17c5","title":"Bouncing Grains Keep Protoplanetary Disks Bright","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"University of Toronto","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Planetesimal; Millimeter; Streaming instability; Wavelength; Planet; Grain size; Accretion (finance); Instability","score_opus":0.007691052680587662,"score_gpt":0.23811734649373026,"score_spread":0.23042629381314259,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417147191","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99816376,0.0003723084,0.00040600725,0.00008312963,0.00001392371,0.0000018995722,0.000019305933,0.00004119082,0.000898531],"genre_scores_gemma":[0.9990625,0.000065778426,0.00019037048,0.00004052514,0.0000043086184,9.756128e-7,0.000023481884,0.000008722285,0.0006033808],"study_design_codex":"bench_or_experimental","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.99990416,0.0000054774614,0.000004061895,0.000024696215,0.000016906124,0.000044671415],"domain_scores_gemma":[0.9994261,0.00010083006,0.0001684203,0.000081824925,0.00005822582,0.00016453408],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009129207,0.00018111961,0.00034171814,0.00023125275,0.0006514774,0.0013532998,0.0003860489,0.0004720103,0.0034448204],"category_scores_gemma":[0.00059833995,0.0002683751,0.0001399129,0.00014616735,0.0006361933,0.00083854294,0.0007243124,0.0005002753,0.00066026556],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084814243,0.0001620336,0.084157184,0.00023905668,0.00011366638,0.001207463,0.0011182248,0.001656379,0.8820881,0.0022177265,0.00084029307,0.025351748],"study_design_scores_gemma":[0.0000822041,0.0010802085,0.820294,0.00010584942,0.00013287082,0.0018018502,0.003679631,0.0053522256,0.14715761,0.0041361046,0.016084384,0.00009309679],"about_ca_topic_score_codex":0.0020917053,"about_ca_topic_score_gemma":0.0023134174,"teacher_disagreement_score":0.0034448204,"about_ca_system_score_codex":0.0003616273,"about_ca_system_score_gemma":0.00015987777,"threshold_uncertainty_score":0.011524081},"labels":[],"label_agreement":null},{"id":"W4417226300","doi":"10.3847/1538-4357/ae10ac","title":"Testing the Origin of Hot Jupiters with Atmospheric Surveys","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astro and Planetary Science","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Montreal Clinical Research Institute; University of Victoria; University of Waterloo","funders":"","keywords":"Hot Jupiter; Planetesimal; Planet; Exoplanet; Population; Context (archaeology); Accretion (finance)","score_opus":0.01274343599477994,"score_gpt":0.22122781338726255,"score_spread":0.2084843773924826,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417226300","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99876773,0.00007068382,0.00045091586,0.000011945767,0.0000021222593,0.0000069677317,0.00011928674,0.000011606138,0.00055880984],"genre_scores_gemma":[0.99914443,0.000021236541,0.0005511188,0.000011380899,0.000004577782,0.0000044789126,0.00016020333,0.0000036514461,0.00009893995],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9996278,0.0000710667,0.000016044134,0.00013431846,0.000071004644,0.00007962623],"domain_scores_gemma":[0.9987644,0.00027567113,0.00046183047,0.00011407616,0.00015174519,0.00023224487],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005063216,0.00021113093,0.0001566737,0.00075829704,0.00046298694,0.0005428984,0.0003762175,0.0002685297,0.0011912754],"category_scores_gemma":[0.0012399997,0.0001600773,0.0001583056,0.0005522023,0.0004892456,0.00045559267,0.0006904911,0.0002216183,0.00017884113],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00015906848,0.00003869742,0.9537091,0.000019885712,0.000040365056,0.00006726858,0.00020205871,0.00018407499,0.041460026,0.00008749988,0.000052418516,0.0039795386],"study_design_scores_gemma":[0.0000036009333,0.00014100329,0.9923103,0.000004487019,0.000018540231,0.00008874818,0.00026759153,0.0007567867,0.0059427964,0.00006321731,0.00039974006,0.0000032786088],"about_ca_topic_score_codex":0.0026159873,"about_ca_topic_score_gemma":0.004329621,"teacher_disagreement_score":0.0026159873,"about_ca_system_score_codex":0.00025141586,"about_ca_system_score_gemma":0.00012165564,"threshold_uncertainty_score":0.0052015185},"labels":[],"label_agreement":null},{"id":"W4417266067","doi":"10.3847/1538-4357/ae1963","title":"Discovery of a Debris Disk around TWA 20","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Montreal Clinical Research Institute; University of Victoria","funders":"Space Telescope Science Institute","keywords":"Debris disk; Debris; RADIUS; Planetary system; Brown dwarf; Orbit (dynamics); Thick disk; Circumstellar disk","score_opus":0.007719743393234451,"score_gpt":0.2297784253632054,"score_spread":0.22205868196997094,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417266067","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9931825,0.00050668116,0.0013887096,0.00013785998,0.000027706688,0.000018325094,0.00032366233,0.00028196993,0.004132683],"genre_scores_gemma":[0.9972134,0.00008835485,0.0013573058,0.00007533773,0.000025900583,0.000009920866,0.000526373,0.000041767293,0.00066153996],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.9998815,0.000005719349,0.0000046281198,0.000034964094,0.000044527744,0.000028528755],"domain_scores_gemma":[0.9996308,0.000029964474,0.000101881975,0.00005638323,0.000051062856,0.00012977427],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00020794536,0.00027910445,0.00032619314,0.0006935638,0.00082164654,0.00083184167,0.000587788,0.0009925857,0.0010284294],"category_scores_gemma":[0.0005658204,0.00022785812,0.0002706938,0.0004640071,0.00038369963,0.0003931541,0.001133347,0.0005175642,0.000708682],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000740343,0.00017530403,0.2509218,0.00028960747,0.0001869782,0.012908225,0.0017957244,0.0015159491,0.68918484,0.002302844,0.0040744506,0.03590387],"study_design_scores_gemma":[0.00008844737,0.0009691684,0.80256563,0.00012250495,0.00018725451,0.011052206,0.0008576736,0.011032024,0.10834168,0.0020867393,0.06261415,0.00008242221],"about_ca_topic_score_codex":0.0014375547,"about_ca_topic_score_gemma":0.0014541951,"teacher_disagreement_score":0.0014375547,"about_ca_system_score_codex":0.0005531979,"about_ca_system_score_gemma":0.00024029391,"threshold_uncertainty_score":0.004013717},"labels":[],"label_agreement":null},{"id":"W4417386364","doi":"10.3847/1538-4357/ae1f18","title":"The SDSS-V Black Hole Mapper Reverberation Mapping Project: Light Echoes of the Coronal-line Region in a Luminous Quasar","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"York University","funders":"","keywords":"Reverberation mapping; RADIUS; Line (geometry); Active galactic nucleus; Luminosity; Emission spectrum; Context (archaeology); Spectral line","score_opus":0.010297670741737883,"score_gpt":0.22698367271362063,"score_spread":0.21668600197188276,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417386364","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9782825,0.00006559226,0.01380884,0.00006481956,0.00001318792,0.000032280455,0.0037054755,0.0017055171,0.0023218081],"genre_scores_gemma":[0.95056254,0.00004462195,0.03826294,0.000032789518,0.000022930846,0.00003015908,0.009076798,0.00046320987,0.0015040769],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99987376,0.000028729042,0.0000036100453,0.000028310762,0.00003780895,0.000027852155],"domain_scores_gemma":[0.9997017,0.000058507703,0.00006270056,0.000059695467,0.000060113427,0.0000573106],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005639862,0.0003360422,0.00016733317,0.0009809597,0.00015767543,0.00033144353,0.00028532092,0.00022149915,0.001728147],"category_scores_gemma":[0.0006771329,0.00010713196,0.00023281177,0.0003998299,0.00011784849,0.00026016062,0.00036437358,0.00014689447,0.00086343545],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0012319682,0.00057683064,0.41673654,0.00019795925,0.0002818488,0.0022439177,0.0026111454,0.029145041,0.2903889,0.0028164608,0.023478394,0.23029104],"study_design_scores_gemma":[0.00007051021,0.00020995324,0.84516776,0.000018901705,0.000046902154,0.0005569543,0.0005858086,0.094933994,0.043639723,0.0012049364,0.013514954,0.000049649032],"about_ca_topic_score_codex":0.0034647454,"about_ca_topic_score_gemma":0.0035742735,"teacher_disagreement_score":0.0034647454,"about_ca_system_score_codex":0.00010083738,"about_ca_system_score_gemma":0.00010221813,"threshold_uncertainty_score":0.0068891644},"labels":[],"label_agreement":null},{"id":"W4417459203","doi":"10.3847/1538-4357/ae182a","title":"Mid-infrared Extinction toward the Galactic Center","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"McGill University; Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"International Space Science Institute; Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency; Simons Foundation","keywords":"Extinction (optical mineralogy); Galactic Center; Spectral line; Line (geometry); Galaxy; Milky Way","score_opus":0.010913666711391988,"score_gpt":0.24833444719926248,"score_spread":0.2374207804878705,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417459203","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.98886395,0.00041096384,0.0024859095,0.000052654468,0.000009798793,0.000009467871,0.000950152,0.00031941893,0.0068977056],"genre_scores_gemma":[0.99802554,0.000070005546,0.0010424213,0.0000359516,0.000009559872,0.000003210155,0.00053858967,0.000021404901,0.00025344698],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99989235,0.000006224202,0.0000031898287,0.00004569352,0.000035009052,0.000017466564],"domain_scores_gemma":[0.9998215,0.000013574433,0.000053969292,0.000019139423,0.000057437028,0.000034338784],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0001871068,0.00031258064,0.00012609393,0.00076001993,0.00026085807,0.00032355275,0.00036716386,0.00016810592,0.0009984096],"category_scores_gemma":[0.0002520627,0.000107610715,0.00020392062,0.00024956424,0.00013338147,0.00029883182,0.00026929064,0.00022151669,0.00051409344],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00016898288,0.00006831837,0.89825785,0.000059709062,0.00016226302,0.00016602704,0.00024165571,0.006168462,0.06574926,0.0013029543,0.0022134795,0.025441043],"study_design_scores_gemma":[0.0000071867853,0.00003087037,0.9813674,0.00001156969,0.000026964368,0.00008346487,0.00005009581,0.0063821343,0.009564778,0.00019088089,0.0022765326,0.000008074811],"about_ca_topic_score_codex":0.008657518,"about_ca_topic_score_gemma":0.0073064226,"teacher_disagreement_score":0.008657518,"about_ca_system_score_codex":0.00048606866,"about_ca_system_score_gemma":0.00009490358,"threshold_uncertainty_score":0.017214239},"labels":[],"label_agreement":null},{"id":"W4417459344","doi":"10.3847/1538-4357/ae1731","title":"SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"Canadian Institute for Theoretical Astrophysics; University of Toronto","funders":"","keywords":"Ophiuchus; Canis; Photometry (optics); Demographics; Range (aeronautics); Astrometry","score_opus":0.010074517313895607,"score_gpt":0.2260709441705259,"score_spread":0.21599642685663029,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W4417459344","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.5323314,0.0016583881,0.0040750266,0.0018057454,0.000644753,0.00037431312,0.17820546,0.0024103795,0.27849448],"genre_scores_gemma":[0.7159265,0.0009709383,0.0046380176,0.00043150983,0.00017761748,0.00034949227,0.11832099,0.0009776584,0.1582073],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9997503,0.000025957535,0.000020123938,0.000061527535,0.00006895227,0.000073002855],"domain_scores_gemma":[0.9993357,0.00008214463,0.00019472573,0.0000715188,0.00012064983,0.00019512819],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0003006043,0.0002621346,0.0002803852,0.0016145532,0.00058412744,0.0010082326,0.00038447455,0.00028130924,0.1286222],"category_scores_gemma":[0.00093128014,0.0000998562,0.00017683397,0.0019528312,0.00019990097,0.00032842424,0.0007104283,0.00025645326,0.056137994],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000593316,0.00019124449,0.42714196,0.0003757838,0.000057988836,0.0014623472,0.00079538825,0.00060584,0.004972967,0.0075787585,0.19948556,0.35673878],"study_design_scores_gemma":[0.00006699162,0.00009732686,0.7313358,0.00015811184,0.000015457967,0.0012818057,0.00056359556,0.00081406505,0.0010244119,0.0014572885,0.26316747,0.000017605198],"about_ca_topic_score_codex":0.014741636,"about_ca_topic_score_gemma":0.009904819,"teacher_disagreement_score":0.1286222,"about_ca_system_score_codex":0.00050254265,"about_ca_system_score_gemma":0.00057275675,"threshold_uncertainty_score":0.43028414},"labels":[],"label_agreement":null},{"id":"W7106678944","doi":"10.3847/1538-4357/ae1745","title":"A Host Galaxy Morphology Link between Quasiperiodic Eruptions and Tidal Disruption Events","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Galaxy; Surface brightness; Galaxy formation and evolution; Population; Galaxy merger; Elliptical galaxy","score_opus":0.008672019548412953,"score_gpt":0.24570942119748213,"score_spread":0.23703740164906917,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7106678944","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9990282,0.000043819884,0.0003707502,0.000024032206,0.0000014266986,0.0000032579999,0.00008303365,0.000013547297,0.0004318959],"genre_scores_gemma":[0.99981636,0.000008922463,0.000077328434,0.0000036085542,0.000002509219,5.251389e-7,0.000050806313,9.245456e-7,0.000039111637],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998616,0.000025566404,0.000010169904,0.00005052743,0.000025988862,0.000026168602],"domain_scores_gemma":[0.99784446,0.0006361145,0.00082988787,0.0002766149,0.000131726,0.00028124897],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00030545637,0.00009229959,0.0001953224,0.00066101266,0.0001957008,0.00081511465,0.00023126113,0.00029913455,0.002228905],"category_scores_gemma":[0.0018791355,0.00014406838,0.00015536233,0.00041804023,0.00037179125,0.00043891478,0.00046940538,0.00024201862,0.00015682107],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00005305769,0.000030641324,0.9948547,0.000006777977,0.00002932567,0.000085209154,0.00006414932,0.00045915853,0.0020728589,0.00025555375,0.000056819652,0.0020317873],"study_design_scores_gemma":[0.0000034178752,0.000021113252,0.9970938,0.0000012291285,0.00000787231,0.00010385094,0.000059516016,0.002263163,0.00017808321,0.00018654668,0.00007974953,0.0000016379247],"about_ca_topic_score_codex":0.0016670433,"about_ca_topic_score_gemma":0.0015095507,"teacher_disagreement_score":0.002228905,"about_ca_system_score_codex":0.00021266539,"about_ca_system_score_gemma":0.0000620731,"threshold_uncertainty_score":0.0074564815},"labels":[],"label_agreement":null},{"id":"W7116854030","doi":"10.3847/1538-4357/ae1d72","title":"Probing a Cosmogenic Origin of Astrophysical Neutrinos and Cosmic Rays Using Gamma-Ray Observations of TXS 0506+056","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Cosmic Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Office of Science; Istituto Nazionale di Fisica Nucleare; High Energy Accelerator Research Organization; National Science Foundation; Agenzia Spaziale Italiana; Japan Aerospace Exploration Agency; U.S. Department of Energy; California Institute of Technology; European Commission; National Energy Research Scientific Computing Center; Jet Propulsion Laboratory; Ministry of Education, Culture, Sports, Science and Technology; National Aeronautics and Space Administration; Natural Sciences and Engineering Research Council of Canada; Smithsonian Institution; Istituto Nazionale di Astrofisica; Institut National de Physique Nucléaire et de Physique des Particules; Vetenskapsrådet","keywords":"Blazar; Neutrino; Intergalactic travel; Cosmic background radiation; Cosmic ray; Cosmic microwave background; Fermi Gamma-ray Space Telescope; Luminosity; Active galactic nucleus; Proton","score_opus":0.022551072707390325,"score_gpt":0.25332479988924006,"score_spread":0.23077372718184974,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7116854030","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9981552,0.000040385992,0.0005542279,0.00002348406,0.0000033774713,0.000008203207,0.00038618132,0.000033989607,0.0007950843],"genre_scores_gemma":[0.99752885,0.000025216277,0.0012287342,0.000015239062,0.000007460041,0.0000039435376,0.0009767086,0.000012448368,0.0002014679],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998221,0.000029627827,0.0000085684815,0.000043738422,0.00006470472,0.000031249616],"domain_scores_gemma":[0.9995672,0.00009562954,0.00013268797,0.000056552446,0.000049317452,0.00009855155],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00066927297,0.00041174423,0.00026887606,0.00060008204,0.0004271338,0.0008153089,0.00032438483,0.0002684959,0.0012164471],"category_scores_gemma":[0.0006840309,0.00022943626,0.00060554914,0.00043193717,0.0002525686,0.00019998792,0.0004320028,0.00038028546,0.00023636717],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0007825532,0.00024897122,0.9152523,0.00004290412,0.00020361332,0.0005114856,0.00031943686,0.012071551,0.06061987,0.0010940562,0.0005625323,0.008290684],"study_design_scores_gemma":[0.00007453528,0.00023446826,0.95103455,0.000019340387,0.000060071547,0.0003542527,0.00013727322,0.03537539,0.010788015,0.0003932777,0.0015088258,0.000019880976],"about_ca_topic_score_codex":0.00957572,"about_ca_topic_score_gemma":0.015552605,"teacher_disagreement_score":0.00957572,"about_ca_system_score_codex":0.00078514544,"about_ca_system_score_gemma":0.00039266265,"threshold_uncertainty_score":0.019039989},"labels":[],"label_agreement":null},{"id":"W7116894655","doi":"10.3847/1538-4357/ae1956","title":"The Radio Afterglow of the Ultralong GRB 220627A","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Gamma-ray bursts and supernovae","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Istituto Nazionale di Astrofisica; University of Toronto; Hebrew University of Jerusalem; Canada Research Chairs; Ministero dell'Università e della Ricerca; Israel Science Foundation; United States - Israel Binational Science Foundation","keywords":"Afterglow; Ejecta; Gamma-ray burst; Redshift; Light curve; Fermi Gamma-ray Space Telescope","score_opus":0.0048623095021251735,"score_gpt":0.2155127285578452,"score_spread":0.21065041905572002,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7116894655","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99801105,0.00019911403,0.00028582872,0.000033719454,0.000011424449,0.000004631028,0.00014130803,0.000029918117,0.0012830948],"genre_scores_gemma":[0.998779,0.000057351866,0.00029176945,0.00004285828,0.000021606287,0.0000047930407,0.00035820436,0.0000074388577,0.00043704567],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9999492,0.0000041730113,0.00000247694,0.000014296212,0.000013102186,0.00001664031],"domain_scores_gemma":[0.99977523,0.000024567269,0.000068419475,0.000032817316,0.000030141124,0.000068806585],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000106995256,0.00017928677,0.0002169276,0.00056225795,0.00032871525,0.00047052742,0.00018743516,0.00035317603,0.0009744272],"category_scores_gemma":[0.0002485235,0.00008233832,0.00014341691,0.00022286788,0.00020510503,0.00018707165,0.0004912042,0.0003198378,0.00041770263],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000695878,0.00027885215,0.6250728,0.00012623865,0.0001203753,0.013264132,0.0006435865,0.0004322538,0.3183064,0.00083614496,0.00151978,0.03870358],"study_design_scores_gemma":[0.00001455569,0.0003319685,0.9792853,0.000016739537,0.000030444333,0.005160153,0.00024388668,0.000580487,0.008966291,0.00015903857,0.0051962915,0.000014775775],"about_ca_topic_score_codex":0.00062641053,"about_ca_topic_score_gemma":0.0009952111,"teacher_disagreement_score":0.0009744272,"about_ca_system_score_codex":0.00011340705,"about_ca_system_score_gemma":0.000045154047,"threshold_uncertainty_score":0.003259778},"labels":[],"label_agreement":null},{"id":"W7116968340","doi":"10.3847/1538-4357/ae22d3","title":"Evidence for Gravitational Lensing in FRB 20190320B: A Potential Lens Mass of ∼420 Solar Masses","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Pulsars and Gravitational Waves Research","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":true,"ca_institutions":"","funders":"","keywords":"Gravitational lens; Redshift; Lens (geology); Strong gravitational lensing; Weak gravitational lensing; Solar mass","score_opus":0.032900932860605595,"score_gpt":0.3606887180918493,"score_spread":0.32778778523124374,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7116968340","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99569327,0.00032959762,0.0007230166,0.00012101837,0.000016179358,0.000012461324,0.0003467881,0.000071536204,0.0026861904],"genre_scores_gemma":[0.9978454,0.00005978829,0.0008888898,0.000064765285,0.000018713157,0.0000056280724,0.0006767414,0.0000164999,0.00042354868],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998318,0.000008929836,0.000006348298,0.000041745378,0.000062469786,0.000048784255],"domain_scores_gemma":[0.999395,0.00006481602,0.0002070032,0.00003624646,0.00008410773,0.00021279063],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00047864116,0.0004279648,0.0003630946,0.0013172351,0.0009770646,0.00091943453,0.00035707344,0.0006065663,0.0021552683],"category_scores_gemma":[0.0007918996,0.00025760135,0.00026312665,0.0009512528,0.0003720059,0.00031128642,0.0006501371,0.00039494876,0.00077424844],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00084975763,0.00013960806,0.78741705,0.00011876143,0.00013701333,0.0025287252,0.0005108657,0.0009346443,0.17666443,0.0019039904,0.002711125,0.026084136],"study_design_scores_gemma":[0.000023905475,0.00010536853,0.99007064,0.000016038666,0.000031859974,0.00062668975,0.0002158818,0.0020815013,0.0036295592,0.00040472974,0.0027794633,0.000014297746],"about_ca_topic_score_codex":0.012931497,"about_ca_topic_score_gemma":0.018784387,"teacher_disagreement_score":0.012931497,"about_ca_system_score_codex":0.00088510464,"about_ca_system_score_gemma":0.0003589915,"threshold_uncertainty_score":0.02571243},"labels":[],"label_agreement":null},{"id":"W7117105705","doi":"10.3847/1538-4357/ae18c8","title":"The White Dwarf Initial–Final Mass Relation from Open Clusters in Gaia DR3","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":2,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada","keywords":"Open cluster; White dwarf; Cluster (spacecraft); Relation (database); Star cluster; Sample (material); Large sample; Stellar mass","score_opus":0.017731528215981295,"score_gpt":0.26645549717687295,"score_spread":0.24872396896089166,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7117105705","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9906617,0.00016036423,0.00082140823,0.000058276655,0.0000055781684,0.000018714438,0.0048318855,0.00008023249,0.0033619492],"genre_scores_gemma":[0.991243,0.000050799954,0.00075538864,0.000031548847,0.000007511309,0.000022878625,0.0070961663,0.000039214414,0.0007534957],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.99971324,0.000025537514,0.000027820714,0.00009482395,0.00007367416,0.000064949716],"domain_scores_gemma":[0.9981091,0.0004801223,0.00050593115,0.00025878238,0.00041621836,0.00022985037],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0005769317,0.00023546182,0.000329835,0.0026724646,0.00051780127,0.00079844234,0.00040076996,0.00022460219,0.001997454],"category_scores_gemma":[0.0026822444,0.00014123118,0.00037127375,0.0026948713,0.0002582215,0.00024579867,0.0010143478,0.0002864163,0.001142177],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0002668111,0.000029440824,0.97701776,0.000060093305,0.00010867574,0.00026672412,0.0008158085,0.0012567325,0.0036004512,0.0011073445,0.0031953966,0.012274851],"study_design_scores_gemma":[0.000004789889,0.000014855693,0.9949214,0.0000088705365,0.000031866803,0.00012589834,0.00027749286,0.000999834,0.00087333703,0.00031040877,0.002422391,0.000008846661],"about_ca_topic_score_codex":0.025690746,"about_ca_topic_score_gemma":0.029712897,"teacher_disagreement_score":0.025690746,"about_ca_system_score_codex":0.0007166714,"about_ca_system_score_gemma":0.00031950563,"threshold_uncertainty_score":0.051082373},"labels":[],"label_agreement":null},{"id":"W7117470291","doi":"10.3847/1538-4357/ae1cc9","title":"Testing the Correlation between Bending Angle and Polarization Properties of Bent Radio Galaxies","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"University of Toronto; Natural Sciences and Engineering Research Council of Canada; Canada Research Chairs; National Science Foundation","keywords":"Faraday effect; Radio galaxy; Polarization (electrochemistry); Linear polarization; Redshift; Faraday cage; Galaxy; Bent molecular geometry","score_opus":0.014042530689702609,"score_gpt":0.2081342237500112,"score_spread":0.1940916930603086,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7117470291","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99889416,0.000019464498,0.00043151272,0.00000893933,0.0000015308303,0.0000019855927,0.00028380792,0.0000114831555,0.00034705194],"genre_scores_gemma":[0.9993038,0.000007983986,0.00015345533,0.000005033147,0.0000028723716,0.0000023285122,0.0004570261,0.0000036617864,0.00006375125],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9992772,0.00019317087,0.000046748686,0.00021575224,0.00012777717,0.00013945723],"domain_scores_gemma":[0.9906481,0.0040183067,0.002791453,0.0009071362,0.00075545174,0.0008796073],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0008523924,0.0002636701,0.00021619252,0.0011512236,0.00024028224,0.00074143667,0.00026079168,0.00031207057,0.0024936302],"category_scores_gemma":[0.0047841114,0.00017368617,0.00025442647,0.00092721486,0.00039356676,0.0003943955,0.0005663408,0.00034477856,0.0005897726],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000046046192,0.000011297598,0.99728405,0.0000029361518,0.000033080192,0.000013930662,0.000023310922,0.00018393446,0.0013581167,0.00002735577,0.000037088357,0.0009789339],"study_design_scores_gemma":[0.0000018176243,0.000024935067,0.99871266,0.0000010437091,0.000008043679,0.00002758842,0.000069777576,0.0006936532,0.0003687912,0.000032126572,0.0000575466,0.0000021194119],"about_ca_topic_score_codex":0.0014267735,"about_ca_topic_score_gemma":0.0012858161,"teacher_disagreement_score":0.0024936302,"about_ca_system_score_codex":0.00012004601,"about_ca_system_score_gemma":0.00008587961,"threshold_uncertainty_score":0.008341968},"labels":[],"label_agreement":null},{"id":"W7117746919","doi":"10.3847/1538-4357/ae1f1a","title":"Warm and Cold Molecular Gas in the Cluster Center of MACS 1931−26 with JWST and ALMA","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Natural Sciences and Engineering Research Council of Canada; Canadian Space Agency","keywords":"Galaxy; Cluster (spacecraft); Galaxy cluster; Star formation; Intergalactic medium; Kinetic energy; Active galactic nucleus; Galactic Center","score_opus":0.0031781078860270095,"score_gpt":0.19504824441019694,"score_spread":0.19187013652416993,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7117746919","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99955624,0.00003156213,0.000041411426,0.000009998882,0.000001215201,0.0000020858715,0.000093251714,0.000009088774,0.00025510276],"genre_scores_gemma":[0.9995573,0.000010465228,0.00010547444,0.000009743165,0.000004864129,0.000002111589,0.00018147586,0.00000332128,0.00012518879],"study_design_codex":"observational","study_design_gemma":"observational","domain_scores_codex":[0.9998716,0.000008891509,0.000004300104,0.000047917016,0.000031770316,0.0000355024],"domain_scores_gemma":[0.9995635,0.000029804345,0.00015856474,0.000048515558,0.000050479768,0.00014904236],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00017416397,0.0002181707,0.00025736028,0.00091634126,0.0004970829,0.00047281722,0.0003925384,0.00018361783,0.0011418958],"category_scores_gemma":[0.00054102886,0.00014735405,0.00021784769,0.0004502128,0.00039361478,0.00028209484,0.0006361161,0.00022159188,0.00021291983],"study_design_candidate":"observational","study_design_consensus":"observational","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.000301414,0.000049217433,0.95409226,0.000012869254,0.00009553904,0.00035867808,0.0004922605,0.00036745484,0.03972219,0.00009818992,0.0003051217,0.00410482],"study_design_scores_gemma":[0.0000034738541,0.000017951026,0.99886,0.0000012728607,0.0000099284,0.00005334583,0.000057946345,0.00020414843,0.00057154003,0.000009565485,0.00020878468,0.000002169053],"about_ca_topic_score_codex":0.03332244,"about_ca_topic_score_gemma":0.044566166,"teacher_disagreement_score":0.03332244,"about_ca_system_score_codex":0.0007323299,"about_ca_system_score_gemma":0.00018250474,"threshold_uncertainty_score":0.066257},"labels":[],"label_agreement":null},{"id":"W7117754132","doi":"10.3847/1538-4357/ae2c75","title":"Photometric Redshift Estimation Using Scaled Ensemble Learning","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Planetary Science Division; Science Mission Directorate; Smithsonian Astrophysical Observatory; Max-Planck-Institut für Astronomie; Toray Science Foundation; High Energy Accelerator Research Organization; National Astronomical Observatory of Japan; National Central University; Max-Planck-Gesellschaft; Department of Atomic Energy, Government of India; Ministry of Education, Culture, Sports, Science and Technology; Queen's University; Cabinet Office, Government of Japan; Eötvös Loránd Tudományegyetem; Academia Sinica; Space Telescope Science Institute; Los Alamos National Laboratory; Princeton University; Johns Hopkins University; Japan Society for the Promotion of Science; Queen's University Belfast; National Aeronautics and Space Administration; Durham University; Japan Science and Technology Agency; Smithsonian Institution; National Science Foundation","keywords":"Photometric redshift; Sky; Boosting (machine learning); Redshift; Galaxy; Large Synoptic Survey Telescope; Ensemble learning; Artificial neural network","score_opus":0.00942038268179887,"score_gpt":0.24481449258060478,"score_spread":0.2353941098988059,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7117754132","genre_codex":"methods","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":null,"domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.13695046,0.00073429296,0.855426,0.00032663232,0.0001501471,0.00006385647,0.00047920857,0.0033365812,0.002532738],"genre_scores_gemma":[0.9093521,0.00017523773,0.08713146,0.00017125606,0.00015345703,0.00004718794,0.0014312316,0.00009200544,0.0014459608],"study_design_codex":"simulation_or_modeling","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9992138,0.00019961958,0.000031750806,0.00022112379,0.00024557303,0.00008798994],"domain_scores_gemma":[0.99800307,0.00060977146,0.00015893714,0.00040915248,0.0007110675,0.000107940716],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0019830624,0.0009564748,0.0012507918,0.0011582639,0.00039635826,0.00092034036,0.0018443819,0.00088296254,0.0012985527],"category_scores_gemma":[0.0046228017,0.00032778518,0.0008139912,0.0008366502,0.00030710708,0.0013866007,0.001255756,0.0012246595,0.0007075146],"study_design_candidate":"simulation_or_modeling","study_design_consensus":"simulation_or_modeling","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00017957449,0.00016502917,0.009002875,0.00003418605,0.00018157849,0.000055118555,0.000034693483,0.7781419,0.002315722,0.0014855211,0.0029546975,0.20544899],"study_design_scores_gemma":[0.0000021373826,0.000009714347,0.00031623946,0.0000018031861,0.0000058459123,0.000004135635,0.0000019800839,0.9986664,0.00030314145,0.0005690215,0.000117404736,0.0000021495125],"about_ca_topic_score_codex":0.007670824,"about_ca_topic_score_gemma":0.0067505375,"teacher_disagreement_score":0.007670824,"about_ca_system_score_codex":0.00059968076,"about_ca_system_score_gemma":0.00062618137,"threshold_uncertainty_score":0.015252352},"labels":[],"label_agreement":null},{"id":"W7117758366","doi":"10.3847/1538-4357/ae29ab","title":"Rotational Spectra and Search for Aromatic Imines: 9-iminofluorene and Benzophenone Imine","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Astrophysics and Star Formation Studies","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Canadian Space Agency; Arnold and Mabel Beckman Foundation","keywords":"Benzophenone; Imine; Molecule; Spectral line; Spectroscopy; Quadrupole; Rotational transition; Diphenylamine","score_opus":0.012680414909822905,"score_gpt":0.2638924737163726,"score_spread":0.2512120588065497,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7117758366","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.99822015,0.00011416011,0.0009085265,0.000026934451,0.0000019469692,0.000004416521,0.00008756333,0.000021190022,0.00061505],"genre_scores_gemma":[0.9987509,0.000032091983,0.001016117,0.000008854522,0.0000015606923,0.0000024494318,0.00006945791,0.0000026158323,0.00011593282],"study_design_codex":"bench_or_experimental","study_design_gemma":"bench_or_experimental","domain_scores_codex":[0.999943,0.0000054738002,0.0000014453906,0.000021788133,0.000014741661,0.000013544168],"domain_scores_gemma":[0.99984026,0.000034682536,0.000069793095,0.000013855739,0.000020103917,0.000021166523],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.000121981,0.0001955365,0.00011716466,0.00042174937,0.00030169418,0.00017126345,0.00032928862,0.00030687,0.001178767],"category_scores_gemma":[0.00019327692,0.00011234,0.00008229193,0.00027892838,0.00018454492,0.0001877566,0.00015715879,0.00022923357,0.0001489701],"study_design_candidate":"bench_or_experimental","study_design_consensus":"bench_or_experimental","about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00020251768,0.00006130491,0.0799815,0.000055856457,0.000023976598,0.00019297558,0.00009698611,0.0013143925,0.91185665,0.000753596,0.00014257245,0.0053176805],"study_design_scores_gemma":[0.000037348913,0.0007518647,0.28286576,0.00002056714,0.00006445717,0.00038811992,0.00030607666,0.032620564,0.67960155,0.0005971858,0.0027159245,0.000030525156],"about_ca_topic_score_codex":0.0012089561,"about_ca_topic_score_gemma":0.0019740749,"teacher_disagreement_score":0.0012089561,"about_ca_system_score_codex":0.00023290301,"about_ca_system_score_gemma":0.00009773096,"threshold_uncertainty_score":0.0039433837},"labels":[],"label_agreement":null},{"id":"W7117783030","doi":"10.3847/1538-4357/ae1446","title":"Scalable Stellar Parameter Inference Using Python-based LASP: From CPU Optimization to GPU Acceleration","year":2025,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Stellar, planetary, and galactic studies","field":"Physics and Astronomy","cited_by":1,"is_retracted":false,"has_abstract":true,"route_ca_aff":false,"route_ca_fund":true,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"","funders":"Lawrence Berkeley National Laboratory; Division of Astronomical Sciences; National Astronomical Observatories, Chinese Academy of Sciences; Science and Technology Facilities Council; University of Colorado Boulder; Instituto de Astrofísica de Canarias; Office of Science; Max-Planck-Institut für Astronomie; Max-Planck-Institut für Astrophysik; National Development and Reform Commission; Commissariat à l'Énergie Atomique et aux Énergies Alternatives; Ministério da Ciência, Tecnologia e Inovação; Smithsonian Institution; U.S. Department of Energy; National Natural Science Foundation of China; Chinese Academy of Sciences; University of Oxford; York University; Leibniz-Gemeinschaft; University of Notre Dame; Carnegie Mellon University; Universidad Nacional Autónoma de México; Alfred P. Sloan Foundation; University of Washington; Johns Hopkins University; Ministerio de Ciencia e Innovación; Carnegie Institution of Washington; University of Utah; Ohio State University; Gordon and Betty Moore Foundation; National Science Foundation; New Mexico State University; University of Portsmouth; Vanderbilt University; Yale University","keywords":"Python (programming language); Inference; Pipeline (software); Scalability; Code refactoring; Parameter space; Residual; Estimation theory; Code (set theory)","score_opus":0.020687574218268008,"score_gpt":0.2626519775114316,"score_spread":0.2419644032931636,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W7117783030","genre_codex":"methods","genre_gemma":"methods","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"methods","genre_consensus":"methods","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.018887693,0.00017772452,0.7900361,0.0004963285,0.0001499422,0.00010072531,0.0023221266,0.18340543,0.0044239345],"genre_scores_gemma":[0.24267077,0.00017366227,0.7157302,0.00093694497,0.00015214486,0.0004164525,0.00771115,0.02782411,0.004384633],"study_design_codex":"design_other","study_design_gemma":"simulation_or_modeling","domain_scores_codex":[0.9986737,0.00028463727,0.00006350159,0.00034458115,0.00048207754,0.00015160846],"domain_scores_gemma":[0.9982253,0.00054477825,0.00012284094,0.00060607656,0.00035470398,0.00014636845],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.0022130378,0.0017028084,0.0010701152,0.00092478294,0.0007970576,0.0018652749,0.004159841,0.0008244008,0.010544045],"category_scores_gemma":[0.007521401,0.0009813341,0.001731571,0.00094409403,0.0011420366,0.002193116,0.003437509,0.0029519799,0.008248333],"study_design_candidate":"simulation_or_modeling","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.0011711038,0.00045032013,0.021376973,0.0009236034,0.0008121462,0.0006722951,0.0007291899,0.3237032,0.03498654,0.04067031,0.15254053,0.42196387],"study_design_scores_gemma":[0.000076269695,0.00003429914,0.0012983845,0.000023187165,0.00002126267,0.00005155884,0.000045390043,0.96261066,0.008058441,0.015726496,0.012008902,0.000045074667],"about_ca_topic_score_codex":0.0077772452,"about_ca_topic_score_gemma":0.009847977,"teacher_disagreement_score":0.010544045,"about_ca_system_score_codex":0.000916339,"about_ca_system_score_gemma":0.0027078846,"threshold_uncertainty_score":0.035273314},"labels":[],"label_agreement":null},{"id":"W764546960","doi":"","title":"Spatially Resolved Imaging at 350 Micrometers of Cold Dust in Nearby Elliptical Galaxies","year":2008,"lang":"en","type":"article","venue":"The Astrophysical Journal","topic":"Galaxies: Formation, Evolution, Phenomena","field":"Physics and Astronomy","cited_by":0,"is_retracted":false,"has_abstract":true,"route_ca_aff":true,"route_ca_fund":false,"route_ca_venue":false,"route_about_ca":false,"ca_institutions":"National Research Council Canada","funders":"","keywords":"Physics; Astrophysics; Galaxy; Astronomy; Elliptical galaxy; Dust lane; Cosmic dust; Star formation; Accretion (finance)","score_opus":0.00889298574390624,"score_gpt":0.20240915404980245,"score_spread":0.1935161683058962,"validation_status":"score_only:v0-immature-baseline","prediction":{"id":"W764546960","genre_codex":"empirical","genre_gemma":"empirical","domain_codex":null,"domain_gemma":null,"model_version":"metacan-v3-hybrid-931329e0061c","genre_candidate":"empirical","genre_consensus":"empirical","domain_candidate":null,"domain_consensus":null,"prediction_status":"machine_predicted_unvalidated","genre_scores_codex":[0.9991351,0.0000772442,0.00023258114,0.000007873094,6.5563677e-7,0.000001849253,0.000058985566,0.000015124828,0.0004706257],"genre_scores_gemma":[0.9987264,0.00003382398,0.0008560529,0.000014975272,0.0000035742744,0.0000032990529,0.00011362493,0.0000030074132,0.00024508135],"study_design_codex":"bench_or_experimental","study_design_gemma":"observational","domain_scores_codex":[0.999943,0.0000033047509,0.0000021282206,0.000019770387,0.000012729806,0.000019026435],"domain_scores_gemma":[0.99980813,0.000026386775,0.000044754233,0.000019191166,0.00002656316,0.000074986776],"candidate_categories":[],"consensus_categories":[],"category_scores_codex":[0.00009119897,0.000107942265,0.0001251703,0.000693427,0.00024243107,0.00022545717,0.0002098805,0.00021624447,0.00055569306],"category_scores_gemma":[0.00017950402,0.0001985712,0.00010731692,0.00020136096,0.00015345335,0.00012827836,0.00027488492,0.00014054053,0.00015936531],"study_design_candidate":"observational","study_design_consensus":null,"about_ca_topic_candidate":false,"about_ca_topic_consensus":false,"about_ca_system_candidate":false,"about_ca_system_consensus":false,"study_design_scores_codex":[0.00036719782,0.00006979446,0.15706733,0.000054380977,0.00003870698,0.0008630248,0.00071724626,0.00038249447,0.82903075,0.00029335386,0.00022704124,0.010888618],"study_design_scores_gemma":[0.000007659324,0.000101958016,0.98943526,0.000004561747,0.000016229378,0.00052300515,0.00014319898,0.0004236227,0.008805616,0.000055112596,0.00047978692,0.000004044407],"about_ca_topic_score_codex":0.0016259351,"about_ca_topic_score_gemma":0.0038268443,"teacher_disagreement_score":0.0016259351,"about_ca_system_score_codex":0.00027759897,"about_ca_system_score_gemma":0.00006205476,"threshold_uncertainty_score":0.003232956},"labels":[],"label_agreement":null}]}